FN Thomson Reuters Web of Science™
VR 1.0
PT J
AU Shrestha, UR
Perera, SMDC
Bhowmik, D
Chawla, U
Mamontov, E
Brown, MF
Chu, XQ
AF Shrestha, Utsab R.
Perera, Suchithranga M. D. C.
Bhowmik, Debsindhu
Chawla, Udeep
Mamontov, Eugene
Brown, Michael F.
Chu, Xiang-Qiang
TI Quasi-elastic Neutron Scattering Reveals Ligand-Induced Protein Dynamics
of a G-Protein-Coupled Receptor
SO JOURNAL OF PHYSICAL CHEMISTRY LETTERS
LA English
DT Article
ID DEEP-SEA HYPERTHERMOPHILE; SMALL-ANGLE NEUTRON; RHODOPSIN ACTIVATION;
POLY(ETHYLENE OXIDE); OLIGOMERIC PROTEIN; AQUEOUS-SOLUTIONS; RELAXATION;
HYDRATION; MOTIONS; NANOPARTICLES
AB Light activation of the visual G-protein-coupled receptor (GPCR) rhodopsin leads to significant structural fluctuations of the protein embedded within the membrane yielding the activation of cognate G-protein (transducin), which initiates biological signaling. Here, we report a quasi-elastic neutron scattering study of the activation of rhodopsin as a GPCR prototype. Our results reveal a broadly distributed relaxation of hydrogen atom dynamics of rhodopsin on a picosecond nanosecond time scale, crucial for protein function, as only observed for globular proteins previously. Interestingly, the results suggest significant differences in the intrinsic protein dynamics of the dark-state rhodopsin versus the ligand-free apoprotein, opsin. These differences can be attributed to the influence of the covalently bound retinal ligand. Furthermore, an idea of the generic free-energy landscape is used to explain the GPCR dynamics of ligand-binding and ligand-free protein conformations, which can be further applied to other GPCR systems.
C1 [Shrestha, Utsab R.; Bhowmik, Debsindhu; Chu, Xiang-Qiang] Wayne State Univ, Dept Phys & Astron, Detroit, MI 48201 USA.
[Perera, Suchithranga M. D. C.; Chawla, Udeep; Brown, Michael F.] Univ Arizona, Dept Chem & Biochem, Tucson, AZ 85721 USA.
[Bhowmik, Debsindhu] Oak Ridge Natl Lab, Computat Sci & Engn Div, Oak Ridge, TN 37831 USA.
[Mamontov, Eugene] Oak Ridge Natl Lab, Chem & Engn Mat Div, Oak Ridge, TN 37831 USA.
[Brown, Michael F.] Univ Arizona, Dept Phys, Tucson, AZ 85721 USA.
RP Chu, XQ (reprint author), Wayne State Univ, Dept Phys & Astron, Detroit, MI 48201 USA.
EM chux@wayne.edu
RI Mamontov, Eugene/Q-1003-2015;
OI Mamontov, Eugene/0000-0002-5684-2675; Chu,
Xiang-qiang/0000-0003-4320-5316
FU Wayne State University; Scientific User Facilities Division, Office of
Basic Energy Sciences, U.S. Department of Energy; U.S. Department of
Energy (DOE) [DE-AC05-00OR22725]; National Science Foundation, Division
of Molecular and Cellular Biosciences (DMCB) [1616008]
FX This work was funded and supported by Wayne State University. The
neutron scattering experiment at the Oak Ridge National Laboratory
(ORNL) Spallation Neutron Source was sponsored by the Scientific User
Facilities Division, Office of Basic Energy Sciences, U.S. Department of
Energy. ORNL is managed by UT Battelle, LLC, for the U.S. Department of
Energy (DOE) under Contract No. DE-AC05-00OR22725. This work is
partially supported by the National Science Foundation, Division of
Molecular and Cellular Biosciences (DMCB), under Grant No. 1616008. We
thank Drs. H. M. O'Neill and Q Zhang of Oak Ridge National Laboratory
for their help during the preparation of the sample environment.
NR 55
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PI WASHINGTON
PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA
SN 1948-7185
J9 J PHYS CHEM LETT
JI J. Phys. Chem. Lett.
PD OCT 20
PY 2016
VL 7
IS 20
BP 4130
EP 4136
DI 10.1021/acsjpclett.6b01632
PG 7
WC Chemistry, Physical; Nanoscience & Nanotechnology; Materials Science,
Multidisciplinary; Physics, Atomic, Molecular & Chemical
SC Chemistry; Science & Technology - Other Topics; Materials Science;
Physics
GA DZ8FP
UT WOS:000386106600016
ER
PT J
AU Yang, C
Hinkle, P
Menestrina, J
Vlassiouk, IV
Siwy, ZS
AF Yang, Crystal
Hinkle, Preston
Menestrina, Justin
Vlassiouk, Ivan V.
Siwy, Zuzanna S.
TI Polarization of Gold in Nanopores Leads to Ion Current Rectification
SO JOURNAL OF PHYSICAL CHEMISTRY LETTERS
LA English
DT Article
ID NANOFLUIDIC DIODE; CONICAL NANOPORES; SURFACE-CHARGE; TRANSISTORS;
TRANSPORT; MEMBRANES; ELECTROOXIDATION; ELECTRODES; NANOTUBES; ETHANOL
AB Biomimetic nanopores with rectifying properties are relevant components of ionic switches, ionic circuits, and biological sensors. Rectification indicates that currents for voltages of one polarity are higher than currents for voltages of the opposite polarity. Ion current rectification requires the presence of surface charges on the pore walls, achieved either by the attachment of charged groups or in multielectrode systems by applying voltage to integrated gate electrodes. Here we present a simpler concept for introducing surface charges via polarization of a thin layer of Au present at one entrance of a silicon nitride nanopore. In an electric field applied by two electrodes placed in bulk solution on both sides of the membrane, the Au layer polarizes such that excess positive charge locally concentrates at one end and negative charge concentrates at the other end. Consequently, a junction is formed between zones with enhanced anion and cation concentrations in the solution adjacent to the Au layer. This bipolar double layer together with enhanced cation concentration in a negatively charged silicon nitride nanopore leads to voltage-controlled surface-charge patterns and ion current rectification. The experimental findings are supported by numerical modeling that confirm modulation of ionic concentrations by the Au layer and ion current rectification even in low-aspect ratio nanopores. Our findings enable a new strategy for creating ionic circuits with diodes and transistors.
C1 [Yang, Crystal; Siwy, Zuzanna S.] Univ Calif Irvine, Dept Chem, Irvine, CA 92697 USA.
[Hinkle, Preston; Menestrina, Justin; Siwy, Zuzanna S.] Univ Calif Irvine, Dept Phys & Astron, Irvine, CA 92697 USA.
[Vlassiouk, Ivan V.] Oak Ridge Natl Lab, 1 Bethel Valley Rd, Oak Ridge, TN 37831 USA.
[Siwy, Zuzanna S.] Univ Calif Irvine, Dept Bioengn, Irvine, CA 92697 USA.
RP Siwy, ZS (reprint author), Univ Calif Irvine, Dept Chem, Irvine, CA 92697 USA.; Siwy, ZS (reprint author), Univ Calif Irvine, Dept Phys & Astron, Irvine, CA 92697 USA.; Siwy, ZS (reprint author), Univ Calif Irvine, Dept Bioengn, Irvine, CA 92697 USA.
EM zsiwy@uci.edu
RI Vlassiouk, Ivan/F-9587-2010
OI Vlassiouk, Ivan/0000-0002-5494-0386
FU National Science Foundation [CHE 1306058]
FX This research was supported by the National Science Foundation (CHE
1306058). Hospitality of the research group of Prof. Meni Wanunu and
training in TEM are greatly acknowledged. We are grateful to Prof. Henry
S. White and Prof. Ulrich F. Keyser for discussions.
NR 49
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PI WASHINGTON
PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA
SN 1948-7185
J9 J PHYS CHEM LETT
JI J. Phys. Chem. Lett.
PD OCT 20
PY 2016
VL 7
IS 20
BP 4152
EP 4158
DI 10.1021/acsjpclett6b01971
PG 7
WC Chemistry, Physical; Nanoscience & Nanotechnology; Materials Science,
Multidisciplinary; Physics, Atomic, Molecular & Chemical
SC Chemistry; Science & Technology - Other Topics; Materials Science;
Physics
GA DZ8FP
UT WOS:000386106600020
ER
PT J
AU Garza, AJ
Scuseria, GE
AF Garza, Alejandro J.
Scuseria, Gustavo E.
TI Predicting Band Gaps with Hybrid Density Functionals
SO JOURNAL OF PHYSICAL CHEMISTRY LETTERS
LA English
DT Article
AB We compare the ability of four popular hybrid density functionals (B3LYP, B3PW91, HSE, and PBE0) for predicting band gaps of semiconductors and insulators over a large benchmark set using a consistent methodology. We observe no significant statistical difference in their overall performance, although the screened hybrid HSE is more accurate for typical semiconductors. HSE can improve its accuracy for large band gap materials-without affecting that of semiconductors-by including a larger portion of Hartree-Fock exchange in its short-range. Given that screened hybrids are computationally much less expensive than their global counterparts, we conclude that they are a better option for the black box prediction of band gaps.
C1 [Garza, Alejandro J.; Scuseria, Gustavo E.] Rice Univ, Dept Chem, POB 1892, Houston, TX 77251 USA.
[Scuseria, Gustavo E.] Rice Univ, Dept Phys & Astron, Houston, TX 77251 USA.
[Garza, Alejandro J.] Lawrence Berkeley Natl Lab, Joint Ctr Artificial Photosynth, Berkeley, CA 94720 USA.
RP Scuseria, GE (reprint author), Rice Univ, Dept Chem, POB 1892, Houston, TX 77251 USA.; Scuseria, GE (reprint author), Rice Univ, Dept Phys & Astron, Houston, TX 77251 USA.
EM guscus@rice.edu
FU Center for the Computational Design of Functional Layered Materials, an
Energy Frontier Research Center - U.S. Department of Energy, Office of
Science, Basic Energy Sciences [DE-SC0012575]; Welch Foundation chair
[C-0036]
FX This work was supported as part of the Center for the Computational
Design of Functional Layered Materials, an Energy Frontier Research
Center funded by the U.S. Department of Energy, Office of Science, Basic
Energy Sciences under Award [# DE-SC0012575]. G.E.S. is a Welch
Foundation chair (C-0036). We also thank the authors of ref 15 for
bringing their paper to our attention and suggesting the use of the
Wilcoxon signed-rank test.
NR 24
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PI WASHINGTON
PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA
SN 1948-7185
J9 J PHYS CHEM LETT
JI J. Phys. Chem. Lett.
PD OCT 20
PY 2016
VL 7
IS 20
BP 4165
EP 4170
DI 10.1021/acs.jpclett.6b01807
PG 6
WC Chemistry, Physical; Nanoscience & Nanotechnology; Materials Science,
Multidisciplinary; Physics, Atomic, Molecular & Chemical
SC Chemistry; Science & Technology - Other Topics; Materials Science;
Physics
GA DZ8FP
UT WOS:000386106600022
ER
PT J
AU Lewis, NHC
Gruenke, NL
Oliver, TAA
Ballottari, M
Bassi, R
Fleming, GR
AF Lewis, Nicholas H. C.
Gruenke, Natalie L.
Oliver, Thomas A. A.
Ballottari, Matteo
Bassi, Roberto
Fleming, Graham R.
TI Observation of Electronic Excitation Transfer Through Light Harvesting
Complex II Using Two-Dimensional Electronic-Vibrational Spectroscopy
SO JOURNAL OF PHYSICAL CHEMISTRY LETTERS
LA English
DT Article
ID ULTRAFAST ENERGY-TRANSFER; HIGHER-PLANTS; LHC-II; CHLOROPHYLL-A; GREEN
PLANTS; PROTEIN; MODEL; PHOTOSYNTHESIS; CAROTENOIDS; TEMPERATURE
AB Light-harvesting complex II (LHCII) serves a central role in light harvesting for oxygenic photosynthesis and is arguably the most important photosynthetic antenna complex. In this work, we present two-dimensional electronic-vibrational (2DEV) spectra of LHCII isolated from spinach, demonstrating the possibility of using this technique to track the transfer of electronic excitation energy between specific pigments within the complex. We assign the spectral bands via comparison with the 2DEV spectra of the isolated chromophores, chlorophyll a and b, and present evidence that excitation energy between the pigments of the complex are observed in these spectra. Finally, we analyze the essential components of the 2DEV spectra using singular value decomposition, which makes it possible to reveal the relaxation pathways within this complex.
C1 [Lewis, Nicholas H. C.; Gruenke, Natalie L.; Oliver, Thomas A. A.; Fleming, Graham R.] Univ Calif Berkeley, Dept Chem, Berkeley, CA 94720 USA.
[Lewis, Nicholas H. C.; Gruenke, Natalie L.; Oliver, Thomas A. A.; Fleming, Graham R.] Lawrence Berkeley Natl Lab, Mol Biophys & Integrated Bioimaging Div, Berkeley, CA 94720 USA.
[Lewis, Nicholas H. C.; Gruenke, Natalie L.; Oliver, Thomas A. A.; Fleming, Graham R.] Kavli Energy Nanosci Inst Berkeley, Berkeley, CA 94720 USA.
[Ballottari, Matteo; Bassi, Roberto] Univ Verona, Fac Sci, Dipartimento Biotecnol, Str Le Grazie, I-37134 Verona, Italy.
[Oliver, Thomas A. A.] Univ Bristol, Sch Chem, Bristol BS8 1TS, Avon, England.
RP Fleming, GR (reprint author), Univ Calif Berkeley, Dept Chem, Berkeley, CA 94720 USA.; Fleming, GR (reprint author), Lawrence Berkeley Natl Lab, Mol Biophys & Integrated Bioimaging Div, Berkeley, CA 94720 USA.; Fleming, GR (reprint author), Kavli Energy Nanosci Inst Berkeley, Berkeley, CA 94720 USA.
EM grfleming@lbl.gov
FU Office of Science, Office of Basic Energy Sciences, U.S. Department of
Energy [DE-AC02-05CH11231]; Division of Chemical Sciences, Geosciences
and Biosciences Division, Office of Basic Energy Sciences (Lawrence
Berkeley National Laboratory and University of California, Berkeley)
[DE-AC03-76F000098]; ERC [679814]
FX This work was supported by the Director, Office of Science, Office of
Basic Energy Sciences, U.S. Department of Energy under Contract
DE-AC02-05CH11231, and the Division of Chemical Sciences, Geosciences
and Biosciences Division, Office of Basic Energy Sciences through Grant
DE-AC03-76F000098 (at Lawrence Berkeley National Laboratory and
University of California, Berkeley). Additionally, this work was
supported by the ERC Starting Grant SOLENALGAE nr 679814 (M.B.).
NR 54
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PI WASHINGTON
PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA
SN 1948-7185
J9 J PHYS CHEM LETT
JI J. Phys. Chem. Lett.
PD OCT 20
PY 2016
VL 7
IS 20
BP 4197
EP 4206
DI 10.1021/acs.jpclett.6b02280
PG 10
WC Chemistry, Physical; Nanoscience & Nanotechnology; Materials Science,
Multidisciplinary; Physics, Atomic, Molecular & Chemical
SC Chemistry; Science & Technology - Other Topics; Materials Science;
Physics
GA DZ8FP
UT WOS:000386106600027
ER
PT J
AU Liu, HY
Naumov, II
Hemley, RJ
AF Liu, Hanyu
Naumov, Ivan I.
Hemley, Russell J.
TI Dense Hydrocarbon Structures at Megabar Pressures
SO JOURNAL OF PHYSICAL CHEMISTRY LETTERS
LA English
DT Article
ID X-RAY-DIFFRACTION; CRYSTAL-STRUCTURE; SOLID HYDROGEN; METHANE; CARBON;
GPA; TEMPERATURES; TRANSITIONS; DIAMOND; SUPERCONDUCTIVITY
AB The structure, bonding, and other properties of phases in the carbon-hydrogen system over a range of conditions are of considerable importance to a broad range of scientific problems. However, the phase diagram of the C-H system at high pressures and temperatures is still not known. To search for new low-energy hydrocarbon structures, we carried out systematic structure prediction calculations for the C-H system from 100 to 300 GPa. We confirmed several previously predicted structures but found additional compositions that adopt more stable structures. In particular, a C2H4 structure is found that has an indirect band gap, and phonon calculations confirm that it is dynamically stable over a broad pressure range. We also identify more carbon-rich structures that are energetically favorable. The results are important for understanding carbon-hydrogen interactions in high-pressure experiments, dense astrophysical environments and the deep carbon cycle in planetary interiors.
C1 [Liu, Hanyu; Naumov, Ivan I.] Carnegie Inst Sci, Geophys Lab, Washington, DC 20015 USA.
[Hemley, Russell J.] George Washington Univ, Dept Civil & Environm Engn, Washington, DC 20052 USA.
[Hemley, Russell J.] Lawrence Livermore Natl Lab, Livermore, CA 94550 USA.
RP Hemley, RJ (reprint author), George Washington Univ, Dept Civil & Environm Engn, Washington, DC 20052 USA.; Hemley, RJ (reprint author), Lawrence Livermore Natl Lab, Livermore, CA 94550 USA.
RI Liu, Hanyu/E-9985-2012
OI Liu, Hanyu/0000-0003-2394-5421
FU EFree, an Energy Frontier Research Center - U.S. Department of Energy,
Office of Science, Office of Basic Energy Sciences [DE-SC0001057]; U.S.
Department of Energy/National Nuclear Security Administration (CDAC)
[DE-NA-0002006]; DOE [DE-AC52-07NA27344]
FX This research was supported by EFree, an Energy Frontier Research Center
funded by the U.S. Department of Energy, Office of Science, Office of
Basic Energy Sciences under Award DE-SC0001057. The infrastructure and
facilities used are supported by the U.S. Department of Energy/National
Nuclear Security Administration (Grant DE-NA-0002006, CDAC). Work at
LLNL was performed under the auspices of the DOE under Contract No.
DE-AC52-07NA27344. This is a contribution to the Deep Carbon
Observatory.
NR 36
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PI WASHINGTON
PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA
SN 1948-7185
J9 J PHYS CHEM LETT
JI J. Phys. Chem. Lett.
PD OCT 20
PY 2016
VL 7
IS 20
BP 4218
EP 4222
DI 10.1021/acs.jpclett.6b02001
PG 5
WC Chemistry, Physical; Nanoscience & Nanotechnology; Materials Science,
Multidisciplinary; Physics, Atomic, Molecular & Chemical
SC Chemistry; Science & Technology - Other Topics; Materials Science;
Physics
GA DZ8FP
UT WOS:000386106600030
ER
PT J
AU Li, SY
Mamo, KA
Yee, HU
AF Li, Shiyong
Mamo, Kiminad A.
Yee, Ho-Ung
TI Jet quenching parameter of the quark-gluon plasma in a strong magnetic
field: Perturbative QCD and AdS/CFT correspondence
SO PHYSICAL REVIEW D
LA English
DT Article
ID RADIATIVE ENERGY-LOSS
AB We compute the jet quenching parameter (q) over cap of a quark-gluon plasma in the presence of a strong magnetic field using perturbative QCD (pQCD) in the weakly coupled regime, and AdS/CFT correspondence in the strongly coupled regime of N = 4 superYang-Mills. In the weakly coupled regime, we compute (q) over cap in pQCD at complete leading order (that is, leading log as well as the constant under the log) in the QCD coupling constant alpha(s), assuming the hierarchy of scales alpha(s)eB << T-2 << eB. We consider two cases of jet orientations with respect to the magnetic field: 1) the case of a jet moving parallel to the magnetic field; 2) the case of a jet moving perpendicular to the magnetic field. In the former case, we find (q) over cap similar to alpha(2)(s)(eB)T log(1/alpha(s)), while in the latter we have (q) over cap similar to alpha(2)(s) (eB)T log(T-2/alpha(s)eB). In both cases, this leading-order result arises from the scatterings with thermally populated lowest-Landau-level quarks. In the strongly coupled regime described by the AdS/CFT correspondence, we find (q) over cap similar to root lambda(eB)T or (q) over cap similar to root lambda root eBT(2) in the same hierarchy of T-2 << eB depending on whether the jet is moving parallel or perpendicular to the magnetic field, respectively, which indicates a universal dependence of (q) over cap on (eB)T in both regimes for the parallel case, the origin of which should be the transverse density of lowest-Landau-level states proportional to eB. Finally, the asymmetric transverse momentum diffusion in the case of a jet moving perpendicular to the magnetic field may give an interesting azimuthal asymmetry of the gluon bremsstrahlung spectrum in the Baier-Dokshitzer-Mueller-Peigne-Schiff and Zakharov (BDMPS-Z) formalism.
C1 [Li, Shiyong; Mamo, Kiminad A.; Yee, Ho-Ung] Univ Illinois, Dept Phys, Chicago, IL 60607 USA.
[Yee, Ho-Ung] Brookhaven Natl Lab, RIKEN BNL Res Ctr, Upton, NY 11973 USA.
RP Li, SY; Mamo, KA; Yee, HU (reprint author), Univ Illinois, Dept Phys, Chicago, IL 60607 USA.; Yee, HU (reprint author), Brookhaven Natl Lab, RIKEN BNL Res Ctr, Upton, NY 11973 USA.
EM sli72@uic.edu; kabebe2@uic.edu; hyee@uic.edu
FU RIKEN-BNL Research Center; U.S. Department of Energy, Office of Science,
Office of Nuclear Physics
FX We thank Tigran Kalaydzhyan, Rob Pisarski, Andrey Sadofyev, and Misha
Stephanov for discussions. We appreciate the hospitality and support
provided by RIKEN-BNL Research Center. This material is based upon work
partially supported by the U.S. Department of Energy, Office of Science,
Office of Nuclear Physics, within the framework of the Beam Energy Scan
Theory (BEST) Topical Collaboration.
NR 21
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U1 2
U2 2
PU AMER PHYSICAL SOC
PI COLLEGE PK
PA ONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA
SN 2470-0010
EI 2470-0029
J9 PHYS REV D
JI Phys. Rev. D
PD OCT 20
PY 2016
VL 94
IS 8
AR 085016
DI 10.1103/PhysRevD.94.085016
PG 20
WC Astronomy & Astrophysics; Physics, Particles & Fields
SC Astronomy & Astrophysics; Physics
GA DZ9DV
UT WOS:000386174700009
ER
PT J
AU Cui, Q
Cheng, JG
Fan, W
Taylor, AE
Calder, S
McGuire, MA
Yan, JQ
Meyers, D
Li, X
Cai, YQ
Jiao, YY
Choi, Y
Haskel, D
Gotou, H
Uwatoko, Y
Chakhalian, J
Christianson, AD
Yunoki, S
Goodenough, JB
Zhou, JS
AF Cui, Q.
Cheng, J. -G.
Fan, W.
Taylor, A. E.
Calder, S.
McGuire, M. A.
Yan, J. -Q.
Meyers, D.
Li, X.
Cai, Y. Q.
Jiao, Y. Y.
Choi, Y.
Haskel, D.
Gotou, H.
Uwatoko, Y.
Chakhalian, J.
Christianson, A. D.
Yunoki, S.
Goodenough, J. B.
Zhou, J. -S.
TI Slater Insulator in Iridate Perovskites with Strong Spin-Orbit Coupling
SO PHYSICAL REVIEW LETTERS
LA English
DT Article
ID SR2IRO4; PHYSICS; OXIDES
AB The perovskite SrIrO3 is an exotic narrow-band metal owing to a confluence of the strengths of the spin-orbit coupling (SOC) and the electron-electron correlations. It has been proposed that topological and magnetic insulating phases can be achieved by tuning the SOC, Hubbard interactions, and/or lattice symmetry. Here, we report that the substitution of nonmagnetic, isovalent Sn4+ for Ir4+ in the SrIr1-xSnxO3 perovskites synthesized under high pressure leads to a metal-insulator transition to an anti-ferromagnetic (AF) phase at T-N >= 225 K. The continuous change of the cell volume as detected by x-ray diffraction and the lambda-shape transition of the specific heat on cooling through T-N demonstrate that the metal-insulator transition is of second order. Neutron powder diffraction results indicate that the Sn substitution enlarges an octahedral-site distortion that reduces the SOC relative to the spin-spin exchange interaction and results in the type-G AF spin ordering below T-N. Measurement of high-temperature magnetic susceptibility shows the evolution of magnetic coupling in the paramagnetic phase typical of weak itinerant-electron magnetism in the Sn-substituted samples. A reduced structural symmetry in the magnetically ordered phase leads to an electron gap opening at the Brillouin zone boundary below T-N in the same way as proposed by Slater.
C1 [Cui, Q.; Cheng, J. -G.; Cai, Y. Q.; Jiao, Y. Y.] Chinese Acad Sci, Beijing Natl Lab Condensed Matter Phys, Beijing 100190, Peoples R China.
[Cui, Q.; Cheng, J. -G.; Cai, Y. Q.; Jiao, Y. Y.] Chinese Acad Sci, Inst Phys, Beijing 100190, Peoples R China.
[Cheng, J. -G.; Li, X.; Goodenough, J. B.; Zhou, J. -S.] Univ Texas Austin, Mat Sci & Engn Program, Austin, TX 78712 USA.
[Fan, W.; Yunoki, S.] RIKEN, Computat Condensed Matter Phys Lab, Wako, Saitama 3510198, Japan.
[Taylor, A. E.; Calder, S.; Christianson, A. D.] Oak Ridge Natl Lab, Quantum Condensed Matter Div, Oak Ridge, TN 37831 USA.
[McGuire, M. A.; Yan, J. -Q.] Oak Ridge Natl Lab, Mat Sci & Technol Div, Oak Ridge, TN 37831 USA.
[Yan, J. -Q.] Univ Tennessee, Dept Mat Sci & Engn, Knoxville, TN 37996 USA.
[Meyers, D.] Univ Arkansas, Dept Phys, Fayetteville, AR 72701 USA.
[Choi, Y.; Haskel, D.] Argonne Natl Lab, Adv Photon Source, Argonne, IL 60439 USA.
[Gotou, H.; Uwatoko, Y.] Univ Tokyo, Inst Solid State Phys, 5-1-5 Kashiwanoha, Chiba 2778581, Japan.
[Chakhalian, J.] Rutgers State Univ, Dept Phys & Astron, 136 Frelinghuysen Rd, Piscataway, NJ 08854 USA.
[Christianson, A. D.] Univ Tennessee, Dept Phys & Astron, Knoxville, TN 37966 USA.
[Yunoki, S.] RIKEN, AICS, Computat Mat Sci Res Team, Kobe, Hyogo 6500047, Japan.
[Yunoki, S.] RIKEN, CEMS, Computat Quantum Matter Res Team, Wako, Saitama 3510198, Japan.
RP Cheng, JG (reprint author), Chinese Acad Sci, Beijing Natl Lab Condensed Matter Phys, Beijing 100190, Peoples R China.; Cheng, JG (reprint author), Chinese Acad Sci, Inst Phys, Beijing 100190, Peoples R China.; Cheng, JG (reprint author), Univ Texas Austin, Mat Sci & Engn Program, Austin, TX 78712 USA.
EM jgcheng@iphy.ac.cn; jszhou@mail.utexas.edu
RI Yunoki, Seiji/B-1831-2008; McGuire, Michael/B-5453-2009
OI McGuire, Michael/0000-0003-1762-9406
FU National Basic Research Program of China [2014CB921500]; National
Science Foundation of China [11304371, 11574377]; Strategic Priority
Research Program of the Chinese Academy of Sciences [XDB 07020100];
Opening Project of Wuhan National High Magnetic Field Center [2015KF22];
Huazhong University of Science and Technology; NSF [DMR-1122603]; Welch
Foundation [F-1066]; U.S. Department of Energy, Office of Science, Basic
Energy Sciences, Materials Science and Engineering Division; Scientific
User Facilities Division; US DOE [DE-AC02-06CH11357]; MEXT Japan
[25287096]
FX This work was supported by the National Basic Research Program of China
(Grant No. 2014CB921500), the National Science Foundation of China
(Grants No. 11304371 and No. 11574377), the Strategic Priority Research
Program of the Chinese Academy of Sciences (Grant No. XDB 07020100), and
the Opening Project of Wuhan National High Magnetic Field Center (Grant
No. 2015KF22), Huazhong University of Science and Technology. J. S. Z.
and J. B. G. were supported by the NSF-DMR-1122603 and the Welch
Foundation (F-1066). The research at Oak Ridge National Laboratory was
supported by the U.S. Department of Energy, Office of Science, Basic
Energy Sciences, Materials Science and Engineering Division (M. A. M.
and J. Q. Y.) and Scientific User Facilities Division (A. E. T., S. C.,
and A. D. C.). Use of the Advanced Photon Source, an Office of Science
User Facility operated for the US DOE, OS by Argonne National
Laboratory, was supported by the US DOE under Contract No.
DE-AC02-06CH11357 (Y. C and D. H.). S. Y. was supported by Grant-in-Aid
for Science Research from MEXT Japan under the Grant No. 25287096.
NR 44
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U1 54
U2 54
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PI COLLEGE PK
PA ONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA
SN 0031-9007
EI 1079-7114
J9 PHYS REV LETT
JI Phys. Rev. Lett.
PD OCT 20
PY 2016
VL 117
IS 17
AR 176603
DI 10.1103/PhysRevLett.117.176603
PG 6
WC Physics, Multidisciplinary
SC Physics
GA EA2AF
UT WOS:000386392700017
PM 27824456
ER
PT J
AU Hirono, Y
Kharzeev, DE
Yin, Y
AF Hirono, Yuji
Kharzeev, Dmitri E.
Yin, Yi
TI Quantized Chiral Magnetic Current from Reconnections of Magnetic Flux
SO PHYSICAL REVIEW LETTERS
LA English
DT Article
ID VIOLATION; HELICITY; MATTER; QCD
AB We introduce a new mechanism for the chiral magnetic effect that does not require an initial chirality imbalance. The chiral magnetic current is generated by reconnections of magnetic flux that change the magnetic helicity of the system. The resulting current is entirely determined by the change of magnetic helicity, and it is quantized.
C1 [Hirono, Yuji; Kharzeev, Dmitri E.; Yin, Yi] Brookhaven Natl Lab, Dept Phys, Upton, NY 11973 USA.
[Kharzeev, Dmitri E.] SUNY Stony Brook, Dept Phys & Astron, Stony Brook, NY 11794 USA.
[Kharzeev, Dmitri E.] Brookhaven Natl Lab, RIKEN BNL Res Ctr, Upton, NY 11973 USA.
RP Hirono, Y (reprint author), Brookhaven Natl Lab, Dept Phys, Upton, NY 11973 USA.
EM yhirono@bnl.gov
FU U.S. Department of Energy, Office of Science, Office of Nuclear Physics
[DEFG-88ER40388, DE-SC0012704]; Beam Energy Scan Theory (BEST) Topical
Collaboration; Japan Society for the Promotion of Science
FX This material is partially based upon work supported by the U.S.
Department of Energy, Office of Science, Office of Nuclear Physics,
under Contracts No. DEFG-88ER40388 (D. K.), No. DE-SC0012704 (Y. H., D.
K., and Y. Y.), and within the framework of the Beam Energy Scan Theory
(BEST) Topical Collaboration. The work of Y. H. was partially supported
by Japan Society for the Promotion of Science Research Fellowships for
Young Scientists. D. K. also acknowledges the support of the Alexander
von Humboldt Foundation and Le Studium foundation, Loire Valley, France,
for the support during the "Condensed matter physics meets relativistic
quantum field theory" program.
NR 26
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U1 3
U2 3
PU AMER PHYSICAL SOC
PI COLLEGE PK
PA ONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA
SN 0031-9007
EI 1079-7114
J9 PHYS REV LETT
JI Phys. Rev. Lett.
PD OCT 20
PY 2016
VL 117
IS 17
AR 172301
DI 10.1103/PhysRevLett.117.172301
PG 5
WC Physics, Multidisciplinary
SC Physics
GA EA2AF
UT WOS:000386392700007
PM 27824439
ER
PT J
AU de Dios, VR
Gessler, A
Ferrio, JP
Alday, JG
Bahn, M
del Castillo, J
Devidal, S
Garcia-Munoz, S
Kayler, Z
Landais, D
Martin-Gomez, P
Milcu, A
Piel, C
Pirhofer-Walzl, K
Ravel, O
Salekin, S
Tissue, DT
Tjoelker, MG
Voltas, J
Roy, J
AF Resco de Dios, Victor
Gessler, Arthur
Pedro Ferrio, Juan
Alday, Josu G.
Bahn, Michael
del Castillo, Jorge
Devidal, Sebastien
Garcia-Munoz, Sonia
Kayler, Zachary
Landais, Damien
Martin-Gomez, Paula
Milcu, Alexandru
Piel, Clement
Pirhofer-Walzl, Karin
Ravel, Olivier
Salekin, Serajis
Tissue, David T.
Tjoelker, Mark G.
Voltas, Jordi
Roy, Jacques
TI Circadian rhythms have significant effects on leaf-to-canopy scale gas
exchange under field conditions
SO GIGASCIENCE
LA English
DT Article
DE Circadian clock; Ecological memory; Net ecosystem exchange; Scaling;
Stomatal conductance models; Photosynthesis; Transpiration
ID CARBON-DIOXIDE EXCHANGE; STOMATAL CONDUCTANCE; WATER-USE;
PHOTOSYNTHESIS; TRANSPIRATION; GROWTH; PLANTS; ASSIMILATION;
ARABIDOPSIS; ATMOSPHERE
AB Background: Molecular clocks drive oscillations in leaf photosynthesis, stomatal conductance, and other cell and leaf-level processes over similar to 24 h under controlled laboratory conditions. The influence of such circadian regulation over whole-canopy fluxes remains uncertain; diurnal CO2 and H2O vapor flux dynamics in the field are currently interpreted as resulting almost exclusively from direct physiological responses to variations in light, temperature and other environmental factors. We tested whether circadian regulation would affect plant and canopy gas exchange at the Montpellier European Ecotron. Canopy and leaf-level fluxes were constantly monitored under field-like environmental conditions, and under constant environmental conditions (no variation in temperature, radiation, or other environmental cues).
Results: We show direct experimental evidence at canopy scales of the circadian regulation of daytime gas exchange: 20-79 % of the daily variation range in CO2 and H2O fluxes occurred under circadian entrainment in canopies of an annual herb (bean) and of a perennial shrub (cotton). We also observed that considering circadian regulation improved performance by 8-17 % in commonly used stomatal conductance models.
Conclusions: Our results show that circadian controls affect diurnal CO2 and H2O flux patterns in entire canopies in field-like conditions, and its consideration significantly improves model performance. Circadian controls act as a 'memory' of the past conditions experienced by the plant, which synchronizes metabolism across entire plant canopies.
C1 [Resco de Dios, Victor; Pedro Ferrio, Juan; Alday, Josu G.; del Castillo, Jorge; Martin-Gomez, Paula; Voltas, Jordi] Univ Lleida, Agrotecn Ctr, Dept Crop & Forest Sci, Lleida 25198, Spain.
[Gessler, Arthur] Swiss Fed Inst Forest Snow & Landscape Res, Long Term Forest Ecosyst Res, CH-8903 Birmensdorf, Switzerland.
[Gessler, Arthur; Kayler, Zachary; Pirhofer-Walzl, Karin] Leibniz Ctr Agr Landscape Res, Inst Landscape Biogeochem, D-15374 Muncheberg, Germany.
[Pedro Ferrio, Juan] Univ Concepcion, Fac Ciencias Nat & Oceanog, Dept Bot, Casilla 160-C, Concepcion, Chile.
[Alday, Josu G.] Univ Liverpool, Sch Environm Sci, Liverpool L69 3GP, Merseyside, England.
[Bahn, Michael] Univ Innsbruck, Inst Ecol, A-6020 Innsbruck, Austria.
[Devidal, Sebastien; Landais, Damien; Milcu, Alexandru; Piel, Clement; Ravel, Olivier; Roy, Jacques] CNRS, Ecotron Europeen Montpellier, UPS 3248, Campus Baillarguet, F-34980 Montferrier Sur Lez, France.
[Garcia-Munoz, Sonia] Inst Madrileno Invest & Desarrollo Rural Agr & Al, Madrid 28800, Spain.
[Kayler, Zachary] US Forest Serv, USDA, Northern Res Stn, Lawrence Livermore Natl Lab, Livermore, CA 94550 USA.
[Milcu, Alexandru] Univ Montpellier, Univ Paul Valery, CNRS, Ctr Ecol Fonct & Evolut,Ecole Prat Hautes Etud,UM, F-34293 Montpellier 5, France.
[Pirhofer-Walzl, Karin] Free Univ Berlin, Inst Biol Plant Ecol, D-14195 Berlin, Germany.
[Pirhofer-Walzl, Karin] Berlin Brandenburg Inst Adv Biodivers Res, D-14195 Berlin, Germany.
[Salekin, Serajis] Univ Lleida, Erasmus Mundus Master Mediterranean Forestry & Na, Lleida 25198, Spain.
[Salekin, Serajis] Univ Canterbury, Coll Engn, Sch Forestry, Christchurch 8140, New Zealand.
[Tissue, David T.; Tjoelker, Mark G.] Univ Western Sydney, Hawkesbury Inst Environm, Richmond, NSW 2753, Australia.
RP de Dios, VR (reprint author), Univ Lleida, Agrotecn Ctr, Dept Crop & Forest Sci, Lleida 25198, Spain.
EM v.rescodedios@gmail.com
RI Gessler, Arthur/C-7121-2008; Ferrio, Juan Pedro/A-5748-2008; Tjoelker,
Mark/M-2413-2016; Alday, Josu G./F-6175-2010; Resco de Dios,
Victor/G-5555-2014
OI Gessler, Arthur/0000-0002-1910-9589; Ferrio, Juan
Pedro/0000-0001-5904-7821; Tjoelker, Mark/0000-0003-4607-5238; Alday,
Josu G./0000-0001-7510-8655; Resco de Dios, Victor/0000-0002-5721-1656
FU Ramon y Cajal fellowships [RYC-2012-10970, RYC-2008-02050]; Leibniz
Centre for Agricultural Landscape Research; Western Sydney University's
Hawkesbury Institute for the Environment; Spanish Government
[AGL2015-69151-R]
FX This study benefited from the CNRS human and technical resources
allocated to the Research Infrastructure Ecotrons, as well as from the
state allocation 'Investissement d'Avenir' ANR-11-INBS-0001; ExpeER
Transnational Access program; Ramon y Cajal fellowships (RYC-2012-10970
to VRD and RYC-2008-02050 to JPF); the Erasmus Mundus Master Course
Mediterranean Forestry and Natural Resources Management (MEDfOR); and
internal grants from the Leibniz Centre for Agricultural Landscape
Research to AG, and from the Western Sydney University's Hawkesbury
Institute for the Environment and the Spanish Government
(AGL2015-69151-R) to VRD.
NR 56
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U1 22
U2 22
PU BIOMED CENTRAL LTD
PI LONDON
PA 236 GRAYS INN RD, FLOOR 6, LONDON WC1X 8HL, ENGLAND
SN 2047-217X
J9 GIGASCIENCE
JI GigaScience
PD OCT 20
PY 2016
VL 5
AR 43
DI 10.1186/s13742-016-0149-y
PG 10
WC Multidisciplinary Sciences
SC Science & Technology - Other Topics
GA DZ1ZH
UT WOS:000385640200001
ER
PT J
AU Day, CJ
King, RM
Shewell, LK
Tram, G
Najnin, T
Hartley-Tassell, LE
Wilson, JC
Fleetwood, AD
Zhulin, IB
Korolik, V
AF Day, Christopher J.
King, Rebecca M.
Shewell, Lucy K.
Tram, Greg
Najnin, Tahria
Hartley-Tassell, Lauren E.
Wilson, Jennifer C.
Fleetwood, Aaron D.
Zhulin, Igor B.
Korolik, Victoria
TI A direct-sensing galactose chemoreceptor recently evolved in invasive
strains of Campylobacter jejuni
SO NATURE COMMUNICATIONS
LA English
DT Article
ID BACILLUS-SUBTILIS; CHEMOTACTIC BEHAVIOR; SIGNAL-TRANSDUCTION; CACO-2
CELLS; AMINO-ACIDS; PROTEIN; IDENTIFICATION; INFECTION; VIRULENCE;
DATABASE
AB A rare chemotaxis receptor, Tlp11, has been previously identified in invasive strains of Campylobacter jejuni, the most prevalent cause of bacterial gastroenteritis worldwide. Here we use glycan and small-molecule arrays, as well as surface plasmon resonance, to show that Tlp11 specifically interacts with galactose. Tlp11 is required for the chemotactic response of C. jejuni to galactose, as shown using wild type, allelic inactivation and addition mutants. The inactivated mutant displays reduced virulence in vivo, in a model of chicken colonization. The Tlp11 sensory domain represents the first known sugar-binding dCache_1 domain, which is the most abundant family of extracellular sensors in bacteria. The Tlp11 signalling domain interacts with the chemotaxis scaffolding proteins CheV and CheW, and comparative genomic analysis indicates a likely recent evolutionary origin for Tlp11. We propose to rename Tlp11 as CcrG, Campylobacter ChemoReceptor for Galactose.
C1 [Day, Christopher J.; King, Rebecca M.; Shewell, Lucy K.; Tram, Greg; Najnin, Tahria; Hartley-Tassell, Lauren E.; Korolik, Victoria] Griffith Univ, Inst Glyc, Gold Coast Campus, Gold Coast, Qld 4222, Australia.
[Wilson, Jennifer C.; Korolik, Victoria] Griffith Univ, Sch Med Sci, Gold Coast Campus, Gold Coast, Qld 4222, Australia.
[Fleetwood, Aaron D.; Zhulin, Igor B.] Univ Tennessee, Dept Microbiol, Knoxville, TN 37996 USA.
[Zhulin, Igor B.] Oak Ridge Natl Lab, Comp Sci & Math Div, Oak Ridge, TN 37861 USA.
RP Korolik, V (reprint author), Griffith Univ, Inst Glyc, Gold Coast Campus, Gold Coast, Qld 4222, Australia.; Korolik, V (reprint author), Griffith Univ, Sch Med Sci, Gold Coast Campus, Gold Coast, Qld 4222, Australia.
EM v.korolik@Griffith.edu.au
OI Zhulin, Igor/0000-0002-6708-5323
FU Institute for Glycomics and School of Medical Science, Griffith
University; NHMRC [1004490]; NIH [R01GM0722285]
FX This work was partially supported by The Institute for Glycomics and
School of Medical Science, Griffith University (V.K.), NH&MRC grant
1004490 (V.K.) and NIH grant R01GM0722285 (I.Z.).
NR 51
TC 0
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U1 8
U2 8
PU NATURE PUBLISHING GROUP
PI LONDON
PA MACMILLAN BUILDING, 4 CRINAN ST, LONDON N1 9XW, ENGLAND
SN 2041-1723
J9 NAT COMMUN
JI Nat. Commun.
PD OCT 20
PY 2016
VL 7
AR 13206
DI 10.1038/ncomms13206
PG 8
WC Multidisciplinary Sciences
SC Science & Technology - Other Topics
GA DZ3FL
UT WOS:000385730500001
PM 27762269
ER
PT J
AU Reid, DR
Lyubimov, I
Ediger, MD
de Pablo, JJ
AF Reid, Daniel R.
Lyubimov, Ivan
Ediger, M. D.
de Pablo, Juan J.
TI Age and structure of a model vapour-deposited glass
SO NATURE COMMUNICATIONS
LA English
DT Article
ID ULTRASTABLE GLASSES; TRANSITION; DYNAMICS; LIQUIDS; POLYSTYRENE;
TEMPERATURE; RELAXATION; STABILITY; CRYSTALS; ORDER
AB Glass films prepared by a process of physical vapour deposition have been shown to have thermodynamic and kinetic stability comparable to those of ordinary glasses aged for thousands of years. A central question in the study of vapour-deposited glasses, particularly in light of new knowledge regarding anisotropy in these materials, is whether the ultra-stable glassy films formed by vapour deposition are ever equivalent to those obtained by liquid cooling. Here we present a computational study of vapour deposition for a two-dimensional glass forming liquid using a methodology, which closely mimics experiment. We find that for the model considered here, structures that arise in vapour-deposited materials are statistically identical to those observed in ordinary glasses, provided the two are compared at the same inherent structure energy. We also find that newly deposited hot molecules produce cascades of hot particles that propagate far into the film, possibly influencing the relaxation of the material.
C1 [Reid, Daniel R.; Lyubimov, Ivan; de Pablo, Juan J.] Univ Chicago, Inst Mol Engn, 5640 South Ellis Ave, Chicago, IL 60637 USA.
[Ediger, M. D.] Univ Wisconsin, Dept Chem, 1101 Univ Ave, Madison, WI 53706 USA.
[de Pablo, Juan J.] Argonne Natl Lab, Inst Mol Engn, 9700 Cass Ave, Lemont, IL 60439 USA.
RP Reid, DR; Lyubimov, I; de Pablo, JJ (reprint author), Univ Chicago, Inst Mol Engn, 5640 South Ellis Ave, Chicago, IL 60637 USA.; Ediger, MD (reprint author), Univ Wisconsin, Dept Chem, 1101 Univ Ave, Madison, WI 53706 USA.; de Pablo, JJ (reprint author), Argonne Natl Lab, Inst Mol Engn, 9700 Cass Ave, Lemont, IL 60439 USA.
EM danielreid@uchicago.edu; ilyubimo@uchicago.edu; ediger@chem.wisc.edu;
depablo@uchicago.edu
FU DMREF grant [NSF-DMR-1234320]; DOE, Basic Energy Sciences, Materials
Research Division, under MICCoM (Midwest Integrated Center for
Computational Materials)
FX We would like to thank David Rodney for many useful conversations. This
work was supported by a DMREF grant NSF-DMR-1234320. Fast
GPU-accelerated codes for simulation of glassy materials were developed
with support from DOE, Basic Energy Sciences, Materials Research
Division, under MICCoM (Midwest Integrated Center for Computational
Materials).
NR 36
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U1 21
U2 21
PU NATURE PUBLISHING GROUP
PI LONDON
PA MACMILLAN BUILDING, 4 CRINAN ST, LONDON N1 9XW, ENGLAND
SN 2041-1723
J9 NAT COMMUN
JI Nat. Commun.
PD OCT 20
PY 2016
VL 7
AR 13062
DI 10.1038/ncomms13062
PG 9
WC Multidisciplinary Sciences
SC Science & Technology - Other Topics
GA DZ3FA
UT WOS:000385729400001
PM 27762262
ER
PT J
AU Zhou, XZ
Smith, BE
Roder, PB
Pauzauskie, PJ
AF Zhou, Xuezhe
Smith, Bennett E.
Roder, Paden B.
Pauzauskie, Peter J.
TI Laser Refrigeration of Ytterbium-Doped Sodium-Yttrium-Fluoride Nanowires
SO ADVANCED MATERIALS
LA English
DT Article
ID STATE OPTICAL REFRIGERATION; UP-CONVERSION; PHOTODYNAMIC THERAPY; FORCE
MICROSCOPY; NANOCRYSTALS; NANOPARTICLES; LUMINESCENCE; CRYSTAL; CELLS;
NANOTRANSDUCERS
AB Sodium yttrium fluoride (beta-NaYF4) nanowires (NWs) with a hexagonal crystal structure are synthesized using a low-cost hydrothermal process and are shown to undergo laser refrigeration based on an upconversion process leading to anti-Stokes (blueshifted) photoluminescence. Single-beam laser trapping combined with forward light scattering is used to investigate cryophotonic laser refrigeration of individual NWs through analysis of their local Brownian dynamics.
C1 [Zhou, Xuezhe; Roder, Paden B.; Pauzauskie, Peter J.] Univ Washington, Dept Mat Sci & Engn, Seattle, WA 98195 USA.
[Smith, Bennett E.] Univ Washington, Dept Chem, Seattle, WA 98195 USA.
[Pauzauskie, Peter J.] Pacific Northwest Natl Lab, Fundamental & Computat Sci Directorate, Richland, WA 99352 USA.
RP Pauzauskie, PJ (reprint author), Univ Washington, Dept Mat Sci & Engn, Seattle, WA 98195 USA.; Pauzauskie, PJ (reprint author), Pacific Northwest Natl Lab, Fundamental & Computat Sci Directorate, Richland, WA 99352 USA.
EM peterpz@uw.edu
FU Air Force Office of Scientific Research Young Investigator Program
[FA95501210400]; University of Washington; US Department of Energy,
Office of Basic Energy Sciences, Synthesis and Processing Program at the
Pacific Northwest National Laboratory [KC0203020-67554]; Department of
Energy by Battelle [DE-AC05-76RL01830]
FX Laser refrigeration research was supported primarily by a grant from the
Air Force Office of Scientific Research Young Investigator Program
(contract #FA95501210400) as well as start-up funding from the
University of Washington. The authors thank Matthew Crane for manuscript
comments and E. James Davis for providing an optical spectrometer with
LN2-cooled detector. Ion exchange experiments were supported
by the US Department of Energy, Office of Basic Energy Sciences,
Synthesis and Processing Program at the Pacific Northwest National
Laboratory (grant #KC0203020-67554). The PNNL is a multiprogram national
laboratory operated for Department of Energy by Battelle under Contract
No. DE-AC05-76RL01830.
NR 43
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U1 44
U2 44
PU WILEY-V C H VERLAG GMBH
PI WEINHEIM
PA POSTFACH 101161, 69451 WEINHEIM, GERMANY
SN 0935-9648
EI 1521-4095
J9 ADV MATER
JI Adv. Mater.
PD OCT 19
PY 2016
VL 28
IS 39
BP 8658
EP 8662
DI 10.1002/adma.201600406
PG 5
WC Chemistry, Multidisciplinary; Chemistry, Physical; Nanoscience &
Nanotechnology; Materials Science, Multidisciplinary; Physics, Applied;
Physics, Condensed Matter
SC Chemistry; Science & Technology - Other Topics; Materials Science;
Physics
GA EB1WO
UT WOS:000387147200010
PM 27514650
ER
PT J
AU Lu, XJ
Wang, YG
Stoumpos, CC
Hu, QY
Guo, XF
Chen, HJ
Yang, LX
Smith, JS
Yang, WG
Zhao, YS
Xu, HW
Kanatzidis, MC
Jia, QX
AF Lu, Xujie
Wang, Yonggang
Stoumpos, Constantinos C.
Hu, Qingyang
Guo, Xiaofeng
Chen, Haijie
Yang, Liuxiang
Smith, Jesse S.
Yang, Wenge
Zhao, Yusheng
Xu, Hongwu
Kanatzidis, Mercouri C.
Jia, Quanxi
TI Enhanced Structural Stability and Photo Responsiveness of CH3NH3SnI3
Perovskite via Pressure-Induced Amorphization and Recrystallization
SO ADVANCED MATERIALS
LA English
DT Article
ID CUBIC BORON-NITRIDE; HYBRID SOLAR-CELLS; HALIDE PEROVSKITES;
PHASE-TRANSITIONS; PERFORMANCE; CH3NH3PBI3; LIGHT; SEMICONDUCTORS;
DEPOSITION; INTERPLAY
AB An organic-inorganic halide CH3NH3SnI3 perovskite with significantly improved structural stability is obtained via pressure-induced amorphization and recrystallization. In situ high-pressure resistance measurements reveal an increased electrical conductivity by 300% in the pressure-treated perovskite. Photocurrent measurements also reveal a substantial enhancement in visible-light responsiveness. The mechanism under lying the enhanced properties is shown to be associated with the pressure-induced structural modification.
C1 [Lu, Xujie; Jia, Quanxi] Los Alamos Natl Lab, Ctr Integrated Nanotechnol, Los Alamos, NM 87545 USA.
[Lu, Xujie; Guo, Xiaofeng; Xu, Hongwu] Los Alamos Natl Lab, Earth & Environm Sci Div, Los Alamos, NM 87545 USA.
[Wang, Yonggang; Zhao, Yusheng] Univ Nevada, High Pressure Sci & Engn Ctr HiPSEC, Las Vegas, NV 89154 USA.
[Wang, Yonggang; Yang, Liuxiang; Yang, Wenge] Carnegie Inst Sci, High Pressure Synerget Consortium HPSynC, Argonne, IL 60439 USA.
[Stoumpos, Constantinos C.; Chen, Haijie; Kanatzidis, Mercouri C.] Northwestern Univ, Dept Chem, Evanston, IL 60208 USA.
[Hu, Qingyang] Carnegie Inst Sci, Geophys Lab, Washington, DC 20015 USA.
[Hu, Qingyang; Yang, Wenge] Ctr High Pressure Sci & Technol Adv Res HPSTAR, Shanghai 201203, Peoples R China.
[Smith, Jesse S.] Carnegie Inst Sci, HPCAT, Argonne, IL 60439 USA.
[Zhao, Yusheng] Southern Univ Sci & Technol, Dept Phys, Shenzhen 518055, Peoples R China.
RP Jia, QX (reprint author), Los Alamos Natl Lab, Ctr Integrated Nanotechnol, Los Alamos, NM 87545 USA.; Xu, HW (reprint author), Los Alamos Natl Lab, Earth & Environm Sci Div, Los Alamos, NM 87545 USA.; Zhao, YS (reprint author), Univ Nevada, High Pressure Sci & Engn Ctr HiPSEC, Las Vegas, NV 89154 USA.; Kanatzidis, MC (reprint author), Northwestern Univ, Dept Chem, Evanston, IL 60208 USA.; Zhao, YS (reprint author), Southern Univ Sci & Technol, Dept Phys, Shenzhen 518055, Peoples R China.
EM zhaoys@sustc.edu.cn; hxu@lanl.gov; m-kanatzidis@northwestern.edu;
qxjia@lanl.gov
RI Lu, Xujie/L-9672-2014;
OI Lu, Xujie/0000-0001-8402-7160; Xu, Hongwu/0000-0002-0793-6923; Wang,
Yonggang/0000-0003-4816-9182
FU Laboratory Directed Research and Development Program of Los Alamos
National Laboratory; DOE/NNSA Center of Excellence [DE-NA0001982,
DE-NA0001974]; DOE-BES [DE-FG02-99ER45775]; NSF; US DOE-BES X-ray
Scattering Core Program [DE-FG02-99ER45775]; NSAF [U1530402]; U.S.
Department of Energy, Office of Science [SC0012541]
FX X.L. acknowledges the J. Robert Oppenheimer Distinguished Fellowship
supported by the Laboratory Directed Research and Development Program of
Los Alamos National Laboratory. The work at Los Alamos National
Laboratory was performed, in part, at the Center for Integrated
Nanotechnologies, an Office of Science User Facility operated for the
U.S. Department of Energy, Office of Science. The UNLV High Pressure
Science and Engineering Center (HiPSEC) is a DOE/NNSA Center of
Excellence supported by Cooperative Agreement DE-NA0001982. HPCAT
operations are supported by DOE NNSA under Award DE-NA0001974 and
DOE-BES under Award DE-FG02-99ER45775, with partial instrumentation
funding by NSF. W.Y. acknowledges the financial support from US DOE-BES
X-ray Scattering Core Program under grant number DE-FG02-99ER45775 and
NSAF(Grant No. U1530402). At Northwestern University, this work was
supported by grant SC0012541 from the U.S. Department of Energy, Office
of Science.
NR 50
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U1 47
U2 47
PU WILEY-V C H VERLAG GMBH
PI WEINHEIM
PA POSTFACH 101161, 69451 WEINHEIM, GERMANY
SN 0935-9648
EI 1521-4095
J9 ADV MATER
JI Adv. Mater.
PD OCT 19
PY 2016
VL 28
IS 39
BP 8663
EP 8668
DI 10.1002/adma.201600771
PG 6
WC Chemistry, Multidisciplinary; Chemistry, Physical; Nanoscience &
Nanotechnology; Materials Science, Multidisciplinary; Physics, Applied;
Physics, Condensed Matter
SC Chemistry; Science & Technology - Other Topics; Materials Science;
Physics
GA EB1WO
UT WOS:000387147200011
PM 27514760
ER
PT J
AU Savage, M
Cheng, YG
Easun, TL
Eyley, JE
Argent, SP
Warren, MR
Lewis, W
Murray, C
Tang, CC
Frogley, MD
Cinque, G
Sun, JL
Rudic, S
Murder, RT
Benham, MJ
Fitch, AN
Blake, AJ
Ramirez-Cuesta, AJ
Yang, SH
Schroder, M
AF Savage, Mathew
Cheng, Yonggiong
Easun, Timothy L.
Eyley, Jennifer E.
Argent, Stephen P.
Warren, Mark R.
Lewis, William
Murray, Claire
Tang, Chiu C.
Frogley, Mark D.
Cinque, Gianfelice
Sun, Junliang
Rudic, Svemir
Murder, Richard T.
Benham, Michael J.
Fitch, Andrew N.
Blake, Alexander J.
Ramirez-Cuesta, Anibal J.
Yang, Sihai
Schroder, Martin
TI Selective Adsorption of Sulfur Dioxide in a Robust Metal-Organic
Framework Material
SO ADVANCED MATERIALS
LA English
DT Article
ID FLUE-GAS IMPURITIES; CARBON-DIOXIDE; CO2 ADSORPTION; POROUS HOST;
STORAGE; HYDROCARBONS; CAPTURE; SEPARATIONS; POLLUTION; HYDROGEN
AB Selective adsorption of SO2 is realized in a porous metal-organic framework material, and in-depth structural and spectroscopic investigations using Xrays, infrared, and neutrons define the underlying interactions that cause SO2 to bind more strongly than CO2 and N-2.
C1 [Savage, Mathew; Eyley, Jennifer E.; Yang, Sihai; Schroder, Martin] Univ Manchester, Sch Chem, Manchester M13 9PL, Lancs, England.
[Cheng, Yonggiong; Ramirez-Cuesta, Anibal J.] Oak Ridge Natl Lab, CEMD, Neutron Sci Directorate, Oak Ridge, TN 37831 USA.
[Easun, Timothy L.] Cardiff Univ, Sch Chem, Cardiff CF10 3XQ, S Glam, Wales.
[Argent, Stephen P.; Lewis, William; Blake, Alexander J.] Univ Nottingham, Sch Chem, Univ Pk, Nottingham NG7 2RD, England.
[Warren, Mark R.; Murray, Claire; Tang, Chiu C.; Frogley, Mark D.; Cinque, Gianfelice] Diamond Light Source, Harwell Sci Campus, Didcot OX11 ODE, Oxon, England.
[Sun, Junliang] Peking Univ, Coll Chem & Mol Engn, Beijing 100871, Peoples R China.
[Rudic, Svemir] STFC Rutherford Appleton Lab, ISIS Neutron & Muon Source, Didcot OX11 0QX, Oxon, England.
[Murder, Richard T.; Benham, Michael J.] Hiden Isochema, 422 Europa Blvd, Warrington WA5 7TS, Cheshire, England.
[Fitch, Andrew N.] European Synchrotron Radiat Facil, F-38043 Grenoble, France.
RP Yang, SH; Schroder, M (reprint author), Univ Manchester, Sch Chem, Manchester M13 9PL, Lancs, England.
EM Sihai.Yang@manchester.ac.uk; M.Schroder@manchester.ac.uk
RI Lewis, William/O-6571-2014; Schroder, Martin/I-5432-2013; Easun,
Timothy/B-9100-2011; Ramirez-Cuesta, Timmy/A-4296-2010;
OI Lewis, William/0000-0001-7103-6981; Schroder,
Martin/0000-0001-6992-0700; Easun, Timothy/0000-0002-0713-2642;
Ramirez-Cuesta, Timmy/0000-0003-1231-0068; Savage,
Mathew/0000-0002-9078-1845
FU University of Manchester; University of Nottingham; EPSRC [EP/I011870,
EP/K038869]; ERC [AdG 226593]; Laboratory Directed Research and
Development program at the Oak Ridge National Laboratory [LDRD 7739]
FX The authors thank the Universities of Manchester and Nottingham for
funding. M.S. acknowledges receipt of funding from EPSRC (EP/I011870;
EP/K038869) and ERC Advanced Grant (AdG 226593). The authors also thank
Dr. C. Muyrn and Dr. J. Waters for their assistance in collecting SEM
(Scanning Electron Microscopy) images. The authors are especially
grateful to STEC and the ISIS Neutron & Muon Source for access to the
TOSCA spectrometer, to Diamond Light Source for access to Beamlines I11,
I19, and B22, to the European Synchrotron Radiation Facility for access
to Beamline ID31 and to ORNL for access to VISION. Computing resources
were made available through the VirtuES (Virtual Experiments in
Spectroscopy) project, funded by Laboratory Directed Research and
Development program (LDRD 7739) at the Oak Ridge National Laboratory.
NR 40
TC 3
Z9 3
U1 64
U2 64
PU WILEY-V C H VERLAG GMBH
PI WEINHEIM
PA POSTFACH 101161, 69451 WEINHEIM, GERMANY
SN 0935-9648
EI 1521-4095
J9 ADV MATER
JI Adv. Mater.
PD OCT 19
PY 2016
VL 28
IS 39
BP 8705
EP 8711
DI 10.1002/adma.201602338
PG 7
WC Chemistry, Multidisciplinary; Chemistry, Physical; Nanoscience &
Nanotechnology; Materials Science, Multidisciplinary; Physics, Applied;
Physics, Condensed Matter
SC Chemistry; Science & Technology - Other Topics; Materials Science;
Physics
GA EB1WO
UT WOS:000387147200017
PM 27529671
ER
PT J
AU Lu, YH
Jiang, ZY
Aydin, K
Verlinde, J
Clothiaux, EE
Botta, G
AF Lu, Yinghui
Jiang, Zhiyuan
Aydin, Kultegin
Verlinde, Johannes
Clothiaux, Eugene E.
Botta, Giovanni
TI A polarimetric scattering database for non-spherical ice particles at
microwave wavelengths
SO ATMOSPHERIC MEASUREMENT TECHNIQUES
LA English
DT Article
ID DISCRETE-DIPOLE APPROXIMATION; AGGREGATE SNOWFLAKES; RADIATIVE-TRANSFER;
RADAR MEASUREMENTS; T-MATRIX; CLOUD; CLASSIFICATION; BACKSCATTERING;
HYDROMETEORS; FREQUENCIES
AB The atmospheric science community has entered a period in which electromagnetic scattering properties at microwave frequencies of realistically constructed ice particles are necessary for making progress on a number of fronts. One front includes retrieval of ice-particle properties and signatures from ground-based, airborne, and satellite-based radar and radiometer observations. Another front is evaluation of model microphysics by application of forward operators to their outputs and comparison to observations during case study periods. Yet a third front is data assimilation, where again forward operators are applied to databases of ice-particle scattering properties and the results compared to observations, with their differences leading to corrections of the model state.
Over the past decade investigators have developed databases of ice-particle scattering properties at microwave frequencies and made them openly available. Motivated by and complementing these earlier efforts, a database containing polarimetric single-scattering properties of various types of ice particles at millimeter to centimeter wavelengths is presented. While the database presented here contains only single-scattering properties of ice particles in a fixed orientation, ice-particle scattering properties are computed for many different directions of the radiation incident on them. These results are useful for understanding the dependence of ice-particle scattering properties on ice-particle orientation with respect to the incident radiation. For ice particles that are small compared to the wavelength, the number of incident directions of the radiation is sufficient to compute reasonable estimates of their (randomly) orientation-averaged scattering properties.
This database is complementary to earlier ones in that it contains complete (polarimetric) scattering property information for each ice particle -44 plates, 30 columns, 405 branched planar crystals, 660 aggregates, and 640 conical graupel - and direction of incident radiation but is limited to four frequencies (X-, Ku-, Ka-, and W-bands), does not include temperature dependencies of the single-scattering properties, and does not include scattering properties averaged over randomly oriented ice particles. Rules for constructing the morphologies of ice particles from one database to the next often differ; consequently, analyses that incorporate all of the different databases will contain the most variability, while illuminating important differences between them. Publication of this database is in support of future analyses of this nature and comes with the hope that doing so helps contribute to the development of a database standard for ice-particle scattering properties, like the NetCDF (Network Common Data Form) CF (Climate and Forecast) or NetCDF CF/Radial metadata conventions.
C1 [Lu, Yinghui; Jiang, Zhiyuan; Verlinde, Johannes; Clothiaux, Eugene E.; Botta, Giovanni] Penn State Univ, Dept Meteorol & Atmospher Sci, University Pk, PA 16802 USA.
[Lu, Yinghui; Aydin, Kultegin; Botta, Giovanni] Penn State Univ, Dept Elect Engn, University Pk, PA 16802 USA.
[Lu, Yinghui] Lawrence Berkeley Natl Lab, Climate & Ecosyst Sci Div, Berkeley, CA USA.
[Botta, Giovanni] Google, New York, NY USA.
RP Aydin, K (reprint author), Penn State Univ, Dept Elect Engn, University Pk, PA 16802 USA.
EM aydin@engr.psu.edu
FU NSF [AGS-128180]; DOE [DE-FG02-05ER64058]; National Science Foundation
FX We would like to thank Giriprakash Palanisamy and Kathy Lazar for their
invaluable help in setting up the database as a Department of Energy
(DOE) Atmospheric Radiation Measurement (ARM) Program Principal
Investigator Data Product that comes with a DOI. Raymond McCord and
Kenneth Kehoe, also of the DOE ARM Program, provided many useful
comments regarding the NetCDF4 files in which the database is housed.
Discussions with Stefan Kneifel, Ralf Bennartz, Alan Geer, Pavlos
Kollias, Ann Fridlind, Greg McFarquhar, Christopher Williams, and
Stephen Nesbit were helpful in framing the scope of the database
products and/or generating interest within the DOE ARM Program in
hosting it. Development of the database was supported primarily by NSF
Grant AGS-128180. Eugene E. Clothiaux's contributions to the database
were supported by DOE Grant DE-FG02-05ER64058. The authors would like to
acknowledge high-performance computing support from Yellowstone
(ark:/85065/d7wd3xhc) provided by NCAR's Computational and Information
Systems Laboratory, sponsored by the National Science Foundation.
Portions of this research were conducted with Advanced
Cyberinfrastructure computational resources provided by the Institute
for CyberScience at The Pennsylvania State University
(http://ics.psu.edu)
NR 59
TC 0
Z9 0
U1 10
U2 10
PU COPERNICUS GESELLSCHAFT MBH
PI GOTTINGEN
PA BAHNHOFSALLEE 1E, GOTTINGEN, 37081, GERMANY
SN 1867-1381
EI 1867-8548
J9 ATMOS MEAS TECH
JI Atmos. Meas. Tech.
PD OCT 19
PY 2016
VL 9
IS 10
BP 5119
EP 5134
DI 10.5194/amt-9-5119-2016
PG 16
WC Meteorology & Atmospheric Sciences
SC Meteorology & Atmospheric Sciences
GA EA4NX
UT WOS:000386590600001
ER
PT J
AU Balram, KC
Westly, DA
Davanco, M
Grutter, KE
Li, Q
Michels, T
Ray, CH
Yu, LY
Kasica, RJ
Wallin, CB
Gilbert, IJ
Bryce, BA
Simelgor, G
Topolancik, J
Lobontiu, N
Liu, YX
Neuzil, P
Svatos, V
Dill, KA
Bertrand, NA
Metzler, MG
Lopez, G
Czaplewski, DA
Ocola, L
Srinivasan, KA
Stavis, SM
Aksyuk, VA
Liddle, JA
Krylov, S
Ilic, BR
AF Balram, Krishna C.
Westly, Daron A.
Davanco, Marcelo
Grutter, Karen E.
Li, Qing
Michels, Thomas
Ray, Christopher H.
Yu, Liya
Kasica, Richard J.
Wallin, Christopher B.
Gilbert, Ian J.
Bryce, Brian A.
Simelgor, Gregory
Topolancik, Juraj
Lobontiu, Nicolae
Liu, Yuxiang
Neuzil, Pavel
Svatos, Vojtech
Dill, Kristen A.
Bertrand, Neal A.
Metzler, Meredith G.
Lopez, Gerald
Czaplewski, David A.
Ocola, Leonidas
Srinivasan, Kartik A.
Stavis, Samuel M.
Aksyuk, Vladimir A.
Liddle, J. Alexander
Krylov, Slava
Ilic, B. Robert
TI The Nanolithography Toolbox
SO JOURNAL OF RESEARCH OF THE NATIONAL INSTITUTE OF STANDARDS AND
TECHNOLOGY
LA English
DT Article
DE CAD; lithography; nanofabrication; nanofluidic; nanophotonic;
nanoplasmonic; nanoscale curved features; nanoscale design; nanoscale
devices
ID ELECTRON-BEAM LITHOGRAPHY; HYDROGEN SILSESQUIOXANE; FABRICATION; DEVICE;
MICROSCOPY; RESOLUTION; RESIST; LINES
AB This article introduces in archival form the Nanolithography Toolbox, a platform-independent software package for scripted lithography pattern layout generation. The Center for Nanoscale Science and Technology (CNST) at the National Institute of Standards and Technology (NIST) developed the Nanolithography Toolbox to help users of the CNST NanoFab design devices with complex curves and aggressive critical dimensions. Using parameterized shapes as building blocks, the Nanolithography Toolbox allows users to rapidly design and layout nanoscale devices of arbitrary complexity through scripting and programming. The Toolbox offers many parameterized shapes, including structure libraries for micro-and nanoelectromechanical systems (MEMS and NEMS) and nanophotonic devices. Furthermore, the Toolbox allows users to precisely define the number of vertices for each shape or create vectorized shapes using Bezier curves. Parameterized control allows users to design smooth curves with complex shapes. The Toolbox is applicable to a broad range of design tasks in the fabrication of microscale and nanoscale devices.
C1 [Balram, Krishna C.; Westly, Daron A.; Davanco, Marcelo; Grutter, Karen E.; Li, Qing; Michels, Thomas; Ray, Christopher H.; Yu, Liya; Kasica, Richard J.; Wallin, Christopher B.; Gilbert, Ian J.; Dill, Kristen A.; Bertrand, Neal A.; Srinivasan, Kartik A.; Stavis, Samuel M.; Aksyuk, Vladimir A.; Liddle, J. Alexander; Ilic, B. Robert] NIST, Gaithersburg, MD 20899 USA.
[Balram, Krishna C.; Li, Qing; Wallin, Christopher B.; Gilbert, Ian J.] Univ Maryland, Maryland NanoCtr, College Pk, MD 20740 USA.
[Bryce, Brian A.] Harvey Mudd Coll, Claremont, CA 91711 USA.
[Simelgor, Gregory] Edico Genome, La Jolla, CA 92037 USA.
[Topolancik, Juraj] Roche Sequencing Solut, Pleasanton, CA 94588 USA.
[Lobontiu, Nicolae] Univ Alaska Anchorage, Mech Engn, Anchorage, AK 99508 USA.
[Liu, Yuxiang] Worcester Polytech Inst, Mech Engn, Worcester, MA 01609 USA.
[Neuzil, Pavel; Svatos, Vojtech] BUT, Cent European Inst Technol CEITEC, Tech 3058 10, CZ-61600 Brno, Czech Republic.
[Neuzil, Pavel] Northwestern Polytech Univ, Dept Microsyst, Xian, Peoples R China.
[Metzler, Meredith G.; Lopez, Gerald] Univ Penn, Quattrone Nanofabricat Facil, Philadelphia, PA 19104 USA.
[Czaplewski, David A.; Ocola, Leonidas] Argonne Natl Lab, Ctr Nanoscale Mat, 9700 S Cass Ave, Argonne, IL 60439 USA.
[Krylov, Slava] Tel Aviv Univ, Sch Mech Engn, IL-69978 Tel Aviv, Israel.
RP Balram, KC (reprint author), NIST, Gaithersburg, MD 20899 USA.; Balram, KC (reprint author), Univ Maryland, Maryland NanoCtr, College Pk, MD 20740 USA.
EM krishna.coimbatorebalram@nist.gov; daron.westly@nist.gov;
marcelo.davanco@nist.gov; karen.grutter.ctr@mail.mil; qing.li@nist.gov;
thomas.michels@nist.gov; christopher.ray@nist.gov; liya.yu@nist.gov;
richard.kasica@nist.gov; christopher.wallin@nist.gov;
ian.gilbert@nist.gov; babryce@gmail.com;
gregory.simelgor@edicogenome.com; juraj.topolancik@roche.com;
nlobontiu@uaa.alaska.edu; yliu11@WPI.EDU; pavel.neuzil@gmail.com;
vojtechsv3@gmail.com; kristen.dill@nist.gov; neal.bertrand@nist.gov;
metzlerm@seas.upenn.edu; lopezg@seas.upenn.edu; dczaplewski@anl.gov;
ocola@anl.gov; kartik.srinivasan@nist.gov; samuel.stavis@nist.gov;
vladimir.aksyuk@nist.gov; liddle@nist.gov; vadis@eng.tau.ac.il;
robert.ilic@nist.gov
RI Liddle, James/A-4867-2013; Neuzil, Pavel/B-9981-2012
OI Liddle, James/0000-0002-2508-7910;
FU University of Maryland; National Institute of Standards and Technology
Center for Nanoscale Science and Technology through the University of
Maryland [70ANB10H193]
FX K.C.B., K.G., Q.L., C.B.W. and I.J.G. acknowledge support under the
Cooperative Research Agreement between the University of Maryland and
the National Institute of Standards and Technology Center for Nanoscale
Science and Technology, award number 70ANB10H193, through the University
of Maryland.
NR 24
TC 2
Z9 2
U1 11
U2 11
PU US GOVERNMENT PRINTING OFFICE
PI WASHINGTON
PA SUPERINTENDENT DOCUMENTS,, WASHINGTON, DC 20402-9325 USA
SN 1044-677X
J9 J RES NATL INST STAN
JI J. Res. Natl. Inst. Stand. Technol.
PD OCT 19
PY 2016
VL 121
BP 464
EP 475
DI 10.6028/jres.121.024
PG 12
WC Instruments & Instrumentation; Physics, Applied
SC Instruments & Instrumentation; Physics
GA EA5DM
UT WOS:000386639600001
ER
PT J
AU Kamke, J
Kittelmann, S
Soni, P
Li, Y
Tavendale, M
Ganesh, S
Janssen, PH
Shi, WB
Froula, J
Rubin, EM
Attwood, GT
AF Kamke, Janine
Kittelmann, Sandra
Soni, Priya
Li, Yang
Tavendale, Michael
Ganesh, Siva
Janssen, Peter H.
Shi, Weibing
Froula, Jeff
Rubin, Edward M.
Attwood, Graeme T.
TI Rumen metagenome and metatranscriptome analyses of low methane yield
sheep reveals a Sharpea-enriched microbiome characterised by lactic acid
formation and utilisation
SO MICROBIOME
LA English
DT Article
DE Bacteria; Metagenomics; Metatranscriptomics; Sheep rumen; Methane;
Lactate production; Lactate utilisation
ID MEGASPHAERA-ELSDENII; SHIKIMATE PATHWAY; METABOLISM; EMISSIONS; LACTATE;
CATTLE; BIOSYNTHESIS; FERMENTATION; PROPIONATE; STRATEGIES
AB Background: Enteric fermentation by farmed ruminant animals is a major source of methane and constitutes the second largest anthropogenic contributor to global warming. Reducing methane emissions from ruminants is needed to ensure sustainable animal production in the future. Methane yield varies naturally in sheep and is a heritable trait that can be used to select animals that yield less methane per unit of feed eaten. We previously demonstrated elevated expression of hydrogenotrophic methanogenesis pathway genes of methanogenic archaea in the rumens of high methane yield (HMY) sheep compared to their low methane yield (LMY) counterparts. Methane production in the rumen is strongly connected to microbial hydrogen production through fermentation processes. In this study, we investigate the contribution that rumen bacteria make to methane yield phenotypes in sheep.
Results: Using deep sequence metagenome and metatranscriptome datasets in combination with 16S rRNA gene amplicon sequencing from HMY and LMY sheep, we show enrichment of lactate-producing Sharpea spp. in LMY sheep bacterial communities. Increased gene and transcript abundances for sugar import and utilisation and production of lactate, propionate and butyrate were also observed in LMY animals. Sharpea azabuensis and Megasphaera spp. act as important drivers of lactate production and utilisation according to phylogenetic analysis and read mappings.
Conclusions: Our findings show that the rumen microbiome in LMY animals supports a rapid heterofermentative growth, leading to lactate production. We postulate that lactate is subsequently metabolised mainly to butyrate in LMY animals, producing 2 mol of hydrogen and 0.5 mol of methane per mol hexose, which represents 24 % less than the 0.66 mol of methane formed from the 2.66 mol of hydrogen produced if hexose fermentation was directly to acetate and butyrate. These findings are consistent with the theory that a smaller rumen size with a higher turnover rate, where rapid heterofermentative growth would be an advantage, results in lower hydrogen production and lower methane formation. Together with previous methanogen gene expression data, this builds a strong concept of how animal traits and microbial communities shape the methane phenotype in sheep.
C1 [Kamke, Janine; Kittelmann, Sandra; Soni, Priya; Li, Yang; Tavendale, Michael; Ganesh, Siva; Janssen, Peter H.; Attwood, Graeme T.] AgResearch Ltd, Grasslands Res Ctr, Tennent Dr, Palmerston North 4442, New Zealand.
[Shi, Weibing; Froula, Jeff; Rubin, Edward M.] Joint Genome Inst, Dept Energy, Walnut Creek, CA 94598 USA.
[Shi, Weibing; Froula, Jeff; Rubin, Edward M.] Lawrence Berkeley Natl Lab, Genom Div, Berkeley, CA 94720 USA.
RP Attwood, GT (reprint author), AgResearch Ltd, Grasslands Res Ctr, Tennent Dr, Palmerston North 4442, New Zealand.
EM graeme.attwood@agresearch.co.nz
OI Tavendale, Michael/0000-0002-8835-7244; Janssen,
Peter/0000-0002-1022-3502
FU New Zealand Fund for Global Partnerships in Livestock Emissions
Research; Office of Science of the US Department of Energy
[DE-AC02-05CH11231]
FX This work was supported by the New Zealand Fund for Global Partnerships
in Livestock Emissions Research, supporting the objectives of the
Livestock Research Group of the Global Research Alliance on Agricultural
Greenhouse Gases. The 16S rRNA gene amplicon sequencing was conducted by
the US Department of Energy Joint Genome Institute which is supported by
the Office of Science of the US Department of Energy under Contract No.
DE-AC02-05CH11231.
NR 50
TC 2
Z9 2
U1 34
U2 34
PU BIOMED CENTRAL LTD
PI LONDON
PA 236 GRAYS INN RD, FLOOR 6, LONDON WC1X 8HL, ENGLAND
SN 2049-2618
J9 MICROBIOME
JI Microbiome
PD OCT 19
PY 2016
VL 4
AR 56
DI 10.1186/s40168-016-0201-2
PG 16
WC Microbiology
SC Microbiology
GA DZ3ET
UT WOS:000385728600002
PM 27760570
ER
PT J
AU Lee, E
Blauwkamp, J
Castro, FC
Wu, JS
Dravid, VP
Yan, PF
Wang, CM
Kim, S
Wolverton, C
Benedek, R
Dogan, F
Park, JS
Croy, JR
Thackeray, MM
AF Lee, Eungje
Blauwkamp, Joel
Castro, Fernando C.
Wu, Jinsong
Dravid, Vinayak P.
Yan, Pengfei
Wang, Chongmin
Kim, Soo
Wolverton, Christopher
Benedek, Roy
Dogan, Fulya
Park, Joong Sun
Croy, Jason R.
Thackeray, Michael M.
TI Exploring Lithium-Cobalt-Nickel Oxide Spinel Electrodes for >= 3.5 V
Li-Ion Cells
SO ACS APPLIED MATERIALS & INTERFACES
LA English
DT Article
DE lithium-ion battery; spinel; lithium-cobalt-nickel oxide; structure;
Stabilizer
ID NUCLEAR-MAGNETIC-RESONANCE; CATHODE MATERIALS; RECHARGEABLE BATTERIES;
MANGANESE OXIDE; CO ELECTRODES; NI; TRANSFORMATION; 400-DEGREES-C;
VOLTAGE; LIXCOO2
AB Recent reports have indicated that a manganese oxide spinel component, when embedded in a relatively small concentration in layered xLi(2)MnO(3)center dot(1-x)LiMO2 (M = Ni, Mn, or Co) electrode systems, can act as a stabilizer that increases their capacity, rate capability, cycle life, and first-cycle efficiency. These findings prompted us to explore the possibility of exploiting lithiated cobalt oxide spinel stabilizers by taking advantage of (1) the low mobility of cobalt ions relative to that of manganese and nickel ions in close-packed oxides and (2) their higher potential (similar to 3.6 V vs Li0) relative to manganese oxide spinels (similar to 2.9 V vs Li0) for the spinel-to-lithiated spinel electrochemical reaction. In particular, we revisited the structural and electrochemical properties of lithiated spinels in the LiCo1-xNixO(2) (0 <= x <= 0.2) system, first reported almost 25 years ago, by means of high-resolution (synchrotron) X-ray diffraction, transmission electron microscopy, nuclear magnetic resonance spectroscopy, electrochemical cell tests, and theoretical calculations. The results provide a deeper understanding of the complexity of intergrown layered/lithiated spinel LiCo1-xNi(x)O(2) structures when prepared in air between 400 and 800 degrees C and the impact of structural variations on their electrochemical behavior. These structures, when used in low concentrations, offer the possibility of improving the cycling stability, energy, and power of high energy (>= 3.5 V) lithium-ion cells.
C1 [Lee, Eungje; Blauwkamp, Joel; Benedek, Roy; Dogan, Fulya; Park, Joong Sun; Croy, Jason R.; Thackeray, Michael M.] Argonne Natl Lab, Chem Sci & Engn Div, Argonne, IL 60439 USA.
[Castro, Fernando C.; Wu, Jinsong; Dravid, Vinayak P.; Kim, Soo; Wolverton, Christopher] Northwestern Univ, Dept Mat Sci & Engn, Evanston, IL 60208 USA.
[Castro, Fernando C.; Wu, Jinsong; Dravid, Vinayak P.] Northwestern Univ, NUANCE Ctr, Evanston, IL 60208 USA.
[Yan, Pengfei; Wang, Chongmin] Pacific Northwest Natl Lab, Environm Mol Sci Lab, Richland, WA 99352 USA.
RP Lee, E; Thackeray, MM (reprint author), Argonne Natl Lab, Chem Sci & Engn Div, Argonne, IL 60439 USA.
EM eungje.lee@anl.gov; thackeray@anl.gov
RI yan, pengfei/E-4784-2016;
OI yan, pengfei/0000-0001-6387-7502; Kim, Soo/0000-0002-1701-6784
FU Advanced Battery Materials Research (BMR) Program; United States
Department of Energy Office of Science laboratory [DE-AC02-06CH11357];
Office of Science of the United States Department of Energy
[DE-AC02-05CH11231]; Northwestern University Argonne Institute of
Science and Engineering (NAISE); Center for Electrochemical Energy
Science (CEES), an Energy Frontier Research Center - United States
Department of Energy, Office of the Science, Basic Energy Science; Soft
and Hybrid Nanotechnology Experimental (SHyNE) Resource [NSF
NNCI-1542205]; MRSEC program at the Materials Research Center [NSF
DMR-1121262]; International Institute for Nanotechnology (TIN); Keck
Foundation; State of Illinois through the IIN; Office of Vehicle
Technologies of the United States Department of Energy
[DE-AC02-05CH11231, 6951379]; DOE's Office of Biological and
Environmental Research; Department of Energy [DE-AC05-76RLO1830]
FX Support from the Advanced Battery Materials Research (BMR) Program, in
particular David Howell and Tien Duong of the United States Department
of Energy, Office of Vehicle Technologies, Energy Efficiency and
Renewable Energy is gratefully acknowledged. The submitted manuscript
was created by UChicago Argonne, LLC, Operator of Argonne National
Laboratory ("Argonne"). Argonne, a United States Department of Energy
Office of Science laboratory, is operated under Contract
DE-AC02-06CH11357. Computer time allocations at the Fusion Computer
Facility, Argonne National Laboratory is gratefully acknowledged. This
research used resources of the National Energy Research Scientific
Computing Center, which is supported by the Office of Science of the
United States Department of Energy under Contract DE-AC02-05CH11231.
S.K. was supported by the Northwestern University Argonne Institute of
Science and Engineering (NAISE), while C.W. was supported as part of the
Center for Electrochemical Energy Science (CEES), an Energy Frontier
Research Center funded by the United States Department of Energy, Office
of the Science, Basic Energy Science. This work made use of the EPIC,
Keck-II, and SPID facilities of the NUANCE Center at Northwestern
University, supported by the Soft and Hybrid Nanotechnology Experimental
(SHyNE) Resource (NSF NNCI-1542205), the MRSEC program (NSF DMR-1121262)
at the Materials Research Center, the International Institute for
Nanotechnology (TIN), the Keck Foundation, and the State of Illinois
through the IIN. Part of the STEM imaging was supported by the Assistant
Secretary for Energy Efficiency and Renewable Energy, Office of Vehicle
Technologies of the United States Department of Energy under Contract
DE-AC02-05CH11231, Subcontract 6951379 (BMR Program), which was
conducted in the William R. Wiley Environmental Molecular Sciences
Laboratory, a national scientific user facility sponsored by the DOE's
Office of Biological and Environmental Research located at Pacific
Northwest National Laboratory (PNNL). PNNL is operated by Battelle for
the Department of Energy under Contract DE-AC05-76RLO1830.
NR 38
TC 0
Z9 0
U1 31
U2 31
PU AMER CHEMICAL SOC
PI WASHINGTON
PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA
SN 1944-8244
J9 ACS APPL MATER INTER
JI ACS Appl. Mater. Interfaces
PD OCT 19
PY 2016
VL 8
IS 41
BP 27720
EP 27729
DI 10.1021/acsami.6b09073
PG 10
WC Nanoscience & Nanotechnology; Materials Science, Multidisciplinary
SC Science & Technology - Other Topics; Materials Science
GA DZ6SO
UT WOS:000385992400035
ER
PT J
AU Karki, K
Huang, YQ
Hwang, S
Gamalski, AD
Whittingham, MS
Zhou, GW
Stach, EA
AF Karki, Khim
Huang, Yiqing
Hwang, Sooyeon
Gamalski, Andrew D.
Whittingham, M. Stanley
Zhou, Guangwen
Stach, Eric A.
TI Tuning the Activity of Oxygen in LiNi0.8Co0.15Al0.05O2 Battery
Electrodes
SO ACS APPLIED MATERIALS & INTERFACES
LA English
DT Article
DE chemical potential; oxidation reduction; transition metal oxides;
lithium-ion battery; transmission electron microscopy
ID LITHIUM-ION BATTERIES; LIXNI0.8CO0.15AL0.05O2 CATHODE MATERIALS;
ENERGY-LOSS SPECTROSCOPY; X-RAY-DIFFRACTION; THERMAL-STABILITY;
STRUCTURAL-CHANGES; IN-SITU; SURFACE; OXIDE; TRANSITION
AB Layered transition metal oxides such as LiNi0.8Co0.15Al0.05O2 (NCA) are highly desirable battery electrodes. However, these materials suffer from thermal runaway caused by deleterious oxygen loss and surface phase transitions when in highly overcharged and overheated conditions, prompting serious safety concerns. Using in situ environmental transmission electron microscopy techniques, we demonstrate that surface oxygen loss and structural changes in the highly overcharged NCA particles are suppressed by exposing them to an oxygen-rich environment. The onset temperature for the loss of oxygen from the electrode particle is delayed to 350 degrees C at oxygen gas overpressure of 400 mTorr. Similar heating of the particles in a reducing hydrogen gas demonstrated a quick onset of oxygen loss at 150 degrees C and rapid surface degradation of the particles. The results reported here illustrate the fundamental mechanism governing the failure processes of electrode particles and highlight possible strategies to circumvent such issues.
C1 [Karki, Khim; Huang, Yiqing; Whittingham, M. Stanley; Zhou, Guangwen] SUNY Binghamton, NECCES, Binghamton, NY 13902 USA.
[Karki, Khim; Hwang, Sooyeon; Gamalski, Andrew D.; Stach, Eric A.] Brookhaven Natl Lab, Ctr Funct Nanomat, Upton, NY 11973 USA.
RP Zhou, GW (reprint author), SUNY Binghamton, NECCES, Binghamton, NY 13902 USA.; Stach, EA (reprint author), Brookhaven Natl Lab, Ctr Funct Nanomat, Upton, NY 11973 USA.
EM gzhou@binghamton.edu; estach@bnl.gov
RI Stach, Eric/D-8545-2011
OI Stach, Eric/0000-0002-3366-2153
FU NorthEast Center for Chemical Energy Storage (NECCES), an Energy
Frontier Research Center - U.S. Department of Energy (DOE), Office of
Science, Basic Energy Sciences [DE-SC0012583]; U.S. DOE Office of
Science Facility, at Brookhaven National Laboratory [DE-SC0012704]
FX This work is supported as part of the NorthEast Center for Chemical
Energy Storage (NECCES), an Energy Frontier Research Center funded by
the U.S. Department of Energy (DOE), Office of Science, Basic Energy
Sciences under Award No. DE-SC0012583. This research used resources of
the Center for Functional Nanomaterials, which is a U.S. DOE Office of
Science Facility, at Brookhaven National Laboratory under Contract No.
DE-SC0012704, which also funded E.A.S.
NR 43
TC 0
Z9 0
U1 54
U2 54
PU AMER CHEMICAL SOC
PI WASHINGTON
PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA
SN 1944-8244
J9 ACS APPL MATER INTER
JI ACS Appl. Mater. Interfaces
PD OCT 19
PY 2016
VL 8
IS 41
BP 27762
EP 27771
DI 10.1021/acsami.6b09585
PG 10
WC Nanoscience & Nanotechnology; Materials Science, Multidisciplinary
SC Science & Technology - Other Topics; Materials Science
GA DZ6SO
UT WOS:000385992400039
ER
PT J
AU Gao, RL
Lu, FC
Zhu, YM
Hahn, MG
Ralph, J
AF Gao, Ruili
Lu, Fachuang
Zhu, Yimin
Hahn, Michael G.
Ralph, John
TI Flexible Method for Conjugation of Phenolic Lignin Model Compounds to
Carrier Proteins
SO JOURNAL OF AGRICULTURAL AND FOOD CHEMISTRY
LA English
DT Article
DE lignin model dimer; lignification; antibody; cBSA-conjugation; NMR
ID TRANSMISSION ELECTRON-MICROSCOPY; PLANT-CELL WALLS; BIOFUEL PRODUCTION;
DOWN-REGULATION; MONOLIGNOL BIOSYNTHESIS; MONOCLONAL-ANTIBODIES;
ARABIDOPSIS-THALIANA; CINNAMOYL-COENZYME; MASS-SPECTROMETRY;
HYDROGEN-BONDS
AB Linking lignin model compounds to carrier proteins is required either to raise antibodies to them or to structurally screen antibodies raised against lignins or models. This paper describes a flexible method to link phenolic compounds of interest to cationic bovine serum albumin (cBSA) without interfering with their important structural features. With the guaiacylglycerol-beta-guaiacyl ether dimer, for example, the linking was accomplished in 89% yield with the number of dimers per carrier protein being as high as 50; NMR experiments on a N-15- and C-13-labeled conjugation product indicated that 13 dimers were added to the native lysine residues and the remainder (similar to 37) to the amine moieties on the ethylenediamine linkers added to BSA; similar to 32% of the available primary amine groups on cBSA were therefore conjugated to the hapten. This loading is suitable for attempting to raise new antibodies to plant lignins and for screening.
C1 [Gao, Ruili; Lu, Fachuang; Ralph, John] Univ Wisconsin, Dept Biochem, Madison, WI 53706 USA.
[Gao, Ruili; Lu, Fachuang; Ralph, John] Univ Wisconsin, Wisconsin Energy Inst, DOE Great Lakes Bioenergy Res Ctr, Madison, WI 53726 USA.
[Zhu, Yimin] Penn State Univ, Altoona Coll, Dept Chem, 3000 Ivyside Pk, Altoona, PA 16601 USA.
[Hahn, Michael G.] Univ Georgia, Complex Carbohydrate Res Ctr, Athens, GA 30602 USA.
RP Gao, RL; Ralph, J (reprint author), Univ Wisconsin, Dept Biochem, Madison, WI 53706 USA.; Gao, RL; Ralph, J (reprint author), Univ Wisconsin, Wisconsin Energy Inst, DOE Great Lakes Bioenergy Res Ctr, Madison, WI 53726 USA.
EM rgao@wisc.edu; jralph@wisc.edu
FU U.S. Department of Energy, Office of Science [BER DOE-DE-SC0006930]
FX We are grateful for funding provided through the U.S. Department of
Energy, Office of Science (BER DOE-DE-SC0006930).
NR 57
TC 0
Z9 0
U1 12
U2 12
PU AMER CHEMICAL SOC
PI WASHINGTON
PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA
SN 0021-8561
EI 1520-5118
J9 J AGR FOOD CHEM
JI J. Agric. Food Chem.
PD OCT 19
PY 2016
VL 64
IS 41
BP 7782
EP 7788
DI 10.1021/acs.jafc.6b04273
PG 7
WC Agriculture, Multidisciplinary; Chemistry, Applied; Food Science &
Technology
SC Agriculture; Chemistry; Food Science & Technology
GA DZ6SJ
UT WOS:000385991900013
ER
PT J
AU Gallington, LC
Kim, IS
Liu, WG
Yakovenko, AA
Platero-Prats, AE
Li, ZY
Wang, TC
Hupp, JT
Farha, OK
Truhlar, DG
Martinson, ABF
Chapman, KW
AF Gallington, Leighanne C.
Kim, In Soo
Liu, Wei-Guang
Yakovenko, Andrey A.
Platero-Prats, Ana E.
Li, Zhanyong
Wang, Timothy C.
Hupp, Joseph T.
Farha, Omar K.
Truhlar, Donald G.
Martinson, Alex B. F.
Chapman, Karena W.
TI Regioselective Atomic Layer Deposition in Metal-Organic Frameworks
Directed by Dispersion Interactions
SO JOURNAL OF THE AMERICAN CHEMICAL SOCIETY
LA English
DT Article
ID AB-INITIO PSEUDOPOTENTIALS; POWDER DIFFRACTION DATA;
TRANSITION-ELEMENTS; BASIS-SETS; MOLECULES; ENVELOPE; CATALYST; MOF
AB The application of atomic layer deposition (ALD) to metal organic frameworks (MOFs) offers a promising new approach to synthesize designer functional materials with atomic precision. While ALD on flat substrates is well established, the complexity of the pore architecture and surface chemistry in MOFs present new challenges. Through in situ synchrotron X-ray powder diffraction, we visualize, how the deposited atoms are localized and redistribute within the MOF during ALD. We demonstrate that the ALD is regioselective, with preferential deposition of oxy-Zn(II) species within the small pores of NU-1000. Complementary density functional calculations indicate that this startling regioselectivity is driven by dispersion interactions associated with the preferential adsorption sites for the organometallic precursors prior to reaction.
C1 [Gallington, Leighanne C.; Yakovenko, Andrey A.; Platero-Prats, Ana E.; Chapman, Karena W.] Argonne Natl Lab, Adv Photon Source, Xray Sci Div, Argonne, IL 60439 USA.
[Kim, In Soo; Martinson, Alex B. F.] Argonne Natl Lab, Div Mat Sci, 9700 S Cass Ave, Argonne, IL 60439 USA.
[Liu, Wei-Guang; Truhlar, Donald G.] Univ Minnesota, Dept Chem, Chem Theory Ctr, 207 Pleasant St SE, Minneapolis, MN 55455 USA.
[Liu, Wei-Guang; Truhlar, Donald G.] Univ Minnesota, Inst Supercomp, Minneapolis, MN 55455 USA.
[Li, Zhanyong; Wang, Timothy C.; Hupp, Joseph T.; Farha, Omar K.] Northwestern Univ, Dept Chem, 2145 Sheridan Rd, Evanston, IL 60208 USA.
[Farha, Omar K.] King Abdulaziz Univ, Fac Sci, Dept Chem, Jeddah 21589, Saudi Arabia.
RP Chapman, KW (reprint author), Argonne Natl Lab, Adv Photon Source, Xray Sci Div, Argonne, IL 60439 USA.
EM chapmank@aps.anl.gov
RI Platero-Prats, Ana Eva/B-2870-2017; Faculty of, Sciences,
KAU/E-7305-2017;
OI Platero-Prats, Ana Eva/0000-0002-2248-2739; Gallington,
Leighanne/0000-0002-0383-7522; Truhlar, Donald/0000-0002-7742-7294
FU Inorganometallic Catalysis Design Center; Energy Frontier Research
Center by the U.S. Department of Energy (DOE), Office of Science, Basic
Energy Sciences [DE-SC0012702]; DOE Office of Science by Argonne
National Laboratory [DE-AC02-06CH11357]; Beatriu de Pinos fellowship
(BP-DGR) from the Catalan Government
FX This work was supported as part of the Inorganometallic Catalysis Design
Center, an Energy Frontier Research Center funded by the U.S. Department
of Energy (DOE), Office of Science, Basic Energy Sciences, under Award
No. DE-SC0012702. It used resources of the Advanced Photon Source, a
U.S. DOE Office of Science User Facility operated for the DOE Office of
Science by Argonne National Laboratory under Contract No.
DE-AC02-06CH11357. A.E.P.-P. acknowledges a Beatriu de Pinos fellowship
(BP-DGR 2014) from the Catalan Government.
NR 23
TC 1
Z9 1
U1 60
U2 60
PU AMER CHEMICAL SOC
PI WASHINGTON
PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA
SN 0002-7863
J9 J AM CHEM SOC
JI J. Am. Chem. Soc.
PD OCT 19
PY 2016
VL 138
IS 41
BP 13513
EP 13516
DI 10.1021/jacs.6b08711
PG 4
WC Chemistry, Multidisciplinary
SC Chemistry
GA DZ6SL
UT WOS:000385992100016
ER
PT J
AU Noriega, R
Barnard, ES
Ursprung, B
Cotts, BL
Penwell, SB
Schuck, PJ
Ginsberg, NS
AF Noriega, Rodrigo
Barnard, Edward S.
Ursprung, Benedikt
Cotts, Benjamin L.
Penwell, Samuel B.
Schuck, P. James
Ginsberg, Naomi S.
TI Uncovering Single-Molecule Photophysical Heterogeneity of Bright,
Thermally Activated Delayed Fluorescence Emitters Dispersed in Glassy
Hosts
SO JOURNAL OF THE AMERICAN CHEMICAL SOCIETY
LA English
DT Article
ID LIGHT-EMITTING-DIODES; HIGH-EFFICIENCY; ROOM-TEMPERATURE; POLYMER
GLASSES; SUPERCOOLED LIQUIDS; ORGANIC-MOLECULES; TRIPLET ENERGY;
METALLIC-GLASS; SILICA GLASS; SPECTROSCOPY
AB Recently developed all-organic emitters used in display applications achieve high brightness by harvesting triplet populations via thermally activated delayed fluorescence. The photophysical properties of these emitters therefore involve new inherent complexities and are strongly affected by interactions with their host material in the solid state. Ensemble measurements occlude the molecular details of how host guest interactions determine fundamental properties such as the essential balance of singlet oscillator strength and triplet harvesting. Therefore, using time-resolved fluorescence spectroscopy, we interrogate these emitters at the single-molecule level and compare their properties in two distinct glassy polymer hosts. We find that nonbonding interactions with, aromatic moieties in the host appear to mediate the molecular configurations of the emitters, but also promote nonradiative quenching pathways. We also find substantial heterogeneity in the time-resolved photoluminescence of these emitters, which is dominated by static disorder in the polymer. Finally, since singlet triplet cycling underpins the mechanism for increased brightness, we present the first room-temperature measurement of singlet triplet equilibration dynamics in this family of emitters. Our observations present a molecular-scale interrogation of host guest interactions in a disordered film, with implications for highly efficient organic light-emitting devices. Combining a single-molecule experimental technique with an emitter that is sensitive to triplet dynamics, yet read out via fluorescence, should also provide a complementary approach to performing fundamental studies of glassy materials over a large dynamic range of time scales.
C1 [Noriega, Rodrigo; Cotts, Benjamin L.; Penwell, Samuel B.; Ginsberg, Naomi S.] Univ Calif Berkeley, Dept Chem, Berkeley, CA 94720 USA.
[Ginsberg, Naomi S.] Univ Calif Berkeley, Dept Phys, Berkeley, CA 94720 USA.
[Noriega, Rodrigo; Ginsberg, Naomi S.] Lawrence Berkeley Natl Lab, Div Mat Sci, Berkeley, CA 94720 USA.
[Barnard, Edward S.; Ursprung, Benedikt; Schuck, P. James] Lawrence Berkeley Natl Lab, Mol Foundry, Berkeley, CA 94720 USA.
[Ginsberg, Naomi S.] Lawrence Berkeley Natl Lab, Mol Biophys & Integrat Bioimaging Div, Berkeley, CA 94720 USA.
[Ginsberg, Naomi S.] Kavli Energy NanoSci Inst, Berkeley, CA 94720 USA.
[Noriega, Rodrigo] Univ Utah, Dept Chem, Salt Lake City, UT 84112 USA.
[Penwell, Samuel B.] Univ Chicago, Dept Chem, 5735 S Ellis Ave, Chicago, IL 60637 USA.
RP Ginsberg, NS (reprint author), Univ Calif Berkeley, Dept Chem, Berkeley, CA 94720 USA.; Ginsberg, NS (reprint author), Univ Calif Berkeley, Dept Phys, Berkeley, CA 94720 USA.; Ginsberg, NS (reprint author), Lawrence Berkeley Natl Lab, Div Mat Sci, Berkeley, CA 94720 USA.; Ginsberg, NS (reprint author), Lawrence Berkeley Natl Lab, Mol Biophys & Integrat Bioimaging Div, Berkeley, CA 94720 USA.; Ginsberg, NS (reprint author), Kavli Energy NanoSci Inst, Berkeley, CA 94720 USA.
EM nsginsberg@berkeley.edu
FU David and Lucile Packard Fellowship for Science and Engineering; Dow
Chemical Company [244699]; Office of Science, Chemical Sciences,
Geosciences, and Biosciences Division, of the U.S. Department of Energy
[DEAC02-05CH1123]; Office of Science, Office of Basic Energy Sciences,
of the U.S. Department of Energy [DE-AC02-05CH11231]; Philomathia
Foundation Postdoctoral Fellowship; Department of Energy Graduate
Research Fellowship [DE-AC05-060R23100]; Alfred P. Sloan Research
Fellowship; National Science Foundation Graduate Research Fellowship
[DGE 1106400]
FX This work has been supported by a David and Lucile Packard Fellowship
for Science and Engineering to N.S.G., by The Dow Chemical Company under
contract #244699, and by the Director, Office of Science, Chemical
Sciences, Geosciences, and Biosciences Division, of the U.S. Department
of Energy under Contract No. DEAC02-05CH1123. Time-resolved fluorescence
experiments at the Lawrence Berkeley Laboratory Molecular Foundry were
performed as part of the Molecular Foundry user program, supported by
the Office of Science, Office of Basic Energy Sciences, of the U.S.
Department of Energy under Contract No. DE-AC02-05CH11231. RN.
acknowledges financial support through a Philomathia Foundation
Postdoctoral Fellowship. S.B.P. acknowledges a Department of Energy
Graduate Research Fellowship (contract no. DE-AC05-060R23100); N.S.G.
acknowledges an Alfred P. Sloan Research Fellowship; B.L.C. acknowledges
a National Science Foundation Graduate Research Fellowship (DGE
1106400).
NR 71
TC 2
Z9 2
U1 34
U2 34
PU AMER CHEMICAL SOC
PI WASHINGTON
PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA
SN 0002-7863
J9 J AM CHEM SOC
JI J. Am. Chem. Soc.
PD OCT 19
PY 2016
VL 138
IS 41
BP 13551
EP 13560
DI 10.1021/jacs.6b05488
PG 10
WC Chemistry, Multidisciplinary
SC Chemistry
GA DZ6SL
UT WOS:000385992100023
ER
PT J
AU Chi, S
Aluru, R
Singh, UR
Liang, RX
Hardy, WN
Bonn, DA
Kreisel, A
Andersen, BM
Nelson, R
Berlijn, T
Ku, W
Hirschfeld, PJ
Wahl, P
AF Chi, Shun
Aluru, Ramakrishna
Singh, Udai Raj
Liang, Ruixing
Hardy, Walter N.
Bonn, D. A.
Kreisel, A.
Andersen, Brian M.
Nelson, R.
Berlijn, T.
Ku, W.
Hirschfeld, P. J.
Wahl, Peter
TI Impact of iron-site defects on superconductivity in LiFeAs
SO PHYSICAL REVIEW B
LA English
DT Article
ID SYMMETRY
AB In conventional s-wave superconductors, only magnetic impurities exhibit impurity bound states, whereas for an s(+/-) order parameter they can occur for both magnetic and nonmagnetic impurities. Impurity bound states in superconductors can thus provide important insight into the order parameter. Here, we present a combined experimental and theoretical study of native and engineered iron-site defects in LiFeAs. A detailed comparison of tunneling spectra measured on impurities with spin-fluctuation theory reveals a continuous evolution from negligible impurity-bound-state features for weaker scattering potential to clearly detectable states for somewhat stronger scattering potentials. All bound states for these intermediate strength potentials are pinned at or close to the gap edge of the smaller gap, a phenomenon that we explain and ascribe to multiorbital physics.
C1 [Chi, Shun; Liang, Ruixing; Hardy, Walter N.; Bonn, D. A.] Univ British Columbia, Dept Phys & Astron, Vancouver, BC V6T 1Z1, Canada.
[Chi, Shun; Liang, Ruixing; Hardy, Walter N.; Bonn, D. A.] Univ British Columbia, Quantum Matter Inst, Vancouver, BC V6T 1Z4, Canada.
[Aluru, Ramakrishna; Singh, Udai Raj; Wahl, Peter] Max Planck Inst Festkorperforsch, Heisenbergstr 1, D-70569 Stuttgart, Germany.
[Aluru, Ramakrishna; Wahl, Peter] Univ St Andrews, Sch Phys & Astron, SUPA, St Andrews KY16 9SS, Fife, Scotland.
[Kreisel, A.; Andersen, Brian M.] Univ Copenhagen, Niels Bohr Inst, Univ Pk 5, DK-2100 Copenhagen, Denmark.
[Nelson, R.] Louisiana State Univ, Dept Phys & Astron, Baton Rouge, LA 70803 USA.
[Berlijn, T.] Oak Ridge Natl Lab, Ctr Nanophase Mat Sci, Oak Ridge, TN 37831 USA.
[Berlijn, T.] Oak Ridge Natl Lab, Comp Sci & Math Div, Oak Ridge, TN 37831 USA.
[Ku, W.] Brookhaven Natl Lab, CMPMSD, Upton, NY 11973 USA.
[Ku, W.] Shanghai Jiao Tong Univ, Dept Phys & Astron, Shanghai 200240, Peoples R China.
[Hirschfeld, P. J.] Univ Florida, Dept Phys, Gainesville, FL 32611 USA.
RP Kreisel, A (reprint author), Univ Copenhagen, Niels Bohr Inst, Univ Pk 5, DK-2100 Copenhagen, Denmark.
EM kreisel@itp.uni-leipzig.de; wahl@st-andrews.ac.uk
RI Wahl, Peter/F-9337-2014; Andersen, Brian /M-4671-2014
OI Wahl, Peter/0000-0002-8635-1519; Andersen, Brian /0000-0002-9786-7553
FU MPG-UBC center; Natural Science and Engineering Research Council of
Canada; Stewart Blusson Quantum Matter Institute; EPSRC [EP/I031014/1];
National Natural Science Foundation of China [11447601]; Ministry of
Science and Technology [2016YFA0300500, 2016YFA0300501]; Lundbeckfond
fellowship [A9318]; [NSF-DMR-1407502]
FX The authors acknowledge useful discussions with C. Hess, Y. Wang, and D.
Guterding. S.C., D.A.B., and P.W. acknowledge funding from the MPG-UBC
center. S.C. and D.A.B. further acknowledge support by the Natural
Science and Engineering Research Council of Canada and the Stewart
Blusson Quantum Matter Institute. P.W. acknowledges financial support
from EPSRC (EP/I031014/1). P.J.H. was supported by Grant No.
NSF-DMR-1407502. A portion of this research was conducted at the Center
for Nanophase Materials Sciences, which is a Department of Energy (DOE)
Office of Science User Facility. W.K. acknowledges support from National
Natural Science Foundation of China Grant No. 11447601 and Ministry of
Science and Technology Grants No. 2016YFA0300500 and No. 2016YFA0300501.
A.K. and B.M.A. acknowledge support from a Lundbeckfond fellowship
(Grant No. A9318). Underpinning data can be obtained at
http://dx.doi.org/10.17630/64f6517a-02e0-407f-8954-cc8f81d4014a.
NR 28
TC 2
Z9 2
U1 9
U2 9
PU AMER PHYSICAL SOC
PI COLLEGE PK
PA ONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA
SN 2469-9950
EI 2469-9969
J9 PHYS REV B
JI Phys. Rev. B
PD OCT 19
PY 2016
VL 94
IS 13
AR 134515
DI 10.1103/PhysRevB.94.134515
PG 6
WC Physics, Condensed Matter
SC Physics
GA DZ8AN
UT WOS:000386090700005
ER
PT J
AU Saglam, H
Zhang, W
Jungfleisch, MB
Sklenar, J
Pearson, JE
Ketterson, JB
Hoffmann, A
AF Saglam, H.
Zhang, W.
Jungfleisch, M. B.
Sklenar, J.
Pearson, J. E.
Ketterson, J. B.
Hoffmann, A.
TI Spin transport through the metallic antiferromagnet FeMn
SO PHYSICAL REVIEW B
LA English
DT Article
ID ROOM-TEMPERATURE; MAGNETIZATION; SPINTRONICS; INJECTION; BILAYER
AB We investigate spin transport through metallic antiferromagnets using measurements based on spin pumping combined with inverse spin Hall effects in Ni80Fe20/FeMn/W trilayers. The relatively large magnitude and opposite sign of spin Hall effects in W compared to FeMn enable an unambiguous detection of spin currents transmitted through the entire FeMn layer thickness. Using this approach we can detect two distinctively different spin transport regimes, which we associate with electronic and magnonic spin currents, respectively. The latter can extend to relatively large distances (approximate to 9 nm) and is enhanced when the antiferromagnetic ordering temperature is close to the measurement temperature.
C1 [Saglam, H.; Zhang, W.; Jungfleisch, M. B.; Sklenar, J.; Pearson, J. E.; Hoffmann, A.] Argonne Natl Lab, Div Mat Sci, Lemont, IL 60439 USA.
[Saglam, H.] IIT, Dept Phys, Chicago, IL 60616 USA.
[Zhang, W.; Ketterson, J. B.] Oakland Univ, Dept Phys, Rochester, MI 48309 USA.
[Sklenar, J.] Northwestern Univ, Dept Phys & Astron, Evanston, IL 60208 USA.
RP Saglam, H (reprint author), Argonne Natl Lab, Div Mat Sci, Lemont, IL 60439 USA.; Saglam, H (reprint author), IIT, Dept Phys, Chicago, IL 60616 USA.
EM saglam@anl.gov; weizhang@oakland.edu; hoffmann@anl.gov
RI Jungfleisch, Matthias Benjamin/G-1069-2015
OI Jungfleisch, Matthias Benjamin/0000-0001-8204-3677
FU U.S. Department of Energy, Office of Science, Basic Energy Sciences,
Materials Science and Engineering Division; DOE, Office of Science,
Basic Energy Sciences [DE-AC02-06CH11357]
FX This work was supported by the U.S. Department of Energy, Office of
Science, Basic Energy Sciences, Materials Science and Engineering
Division. Lithographic patterning was carried out at the Center for
Nanoscale Materials, which is supported by the DOE, Office of Science,
Basic Energy Sciences under Contract No. DE-AC02-06CH11357.
NR 44
TC 1
Z9 1
U1 22
U2 22
PU AMER PHYSICAL SOC
PI COLLEGE PK
PA ONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA
SN 2469-9950
EI 2469-9969
J9 PHYS REV B
JI Phys. Rev. B
PD OCT 19
PY 2016
VL 94
IS 14
AR 140412
DI 10.1103/PhysRevB.94.140412
PG 5
WC Physics, Condensed Matter
SC Physics
GA DZ8BU
UT WOS:000386094400001
ER
PT J
AU Sato, TJ
Okuyama, D
Hong, T
Kikkawa, A
Taguchi, Y
Arima, T
Tokura, Y
AF Sato, Taku J.
Okuyama, Daisuke
Hong, Tao
Kikkawa, Akiko
Taguchi, Yasujiro
Arima, Taka-hisa
Tokura, Yoshinori
TI Magnon dispersion shift in the induced ferromagnetic phase of
noncentrosymmetric MnSi
SO PHYSICAL REVIEW B
LA English
DT Article
ID DZYALOSHINSKII-MORIYA INTERACTION; SPIN-DENSITY-WAVE; SCATTERING;
EXCHANGE
AB A small angle neutron inelastic scattering measurement has been performed to study the magnon dispersion relation in the field-induced ferromagnetic phase of the noncentrosymmetric binary compound MnSi. For the magnons propagating parallel or antiparallel to the external magnetic field, we experimentally confirmed that the dispersion relation is asymmetrically shifted along the magnetic field direction. This magnon dispersion shift is attributed to the relativistic Dzyaloshinskii-Moriya interaction, which is finite in noncentrosymmetric magnets, such as MnSi. The shift direction is found to be switchable by reversing the external magnetic field direction.
C1 [Sato, Taku J.; Okuyama, Daisuke] Tohoku Univ, Inst Multidisciplinary Res Adv Mat, 2-1-1 Katahira, Sendai, Miyagi 9808577, Japan.
[Hong, Tao] Oak Ridge Natl Lab, Quantum Condensed Matter Div, Oak Ridge, TN 37831 USA.
[Kikkawa, Akiko; Taguchi, Yasujiro; Arima, Taka-hisa; Tokura, Yoshinori] RIKEN Ctr Emergent Matter Sci CEMS, Wako, Saitama 3510198, Japan.
[Arima, Taka-hisa] Univ Tokyo, Dept Adv Mat Sci, Kashiwa, Chiba 2778561, Japan.
[Tokura, Yoshinori] Univ Tokyo, Dept Appl Phys, Tokyo 1138656, Japan.
[Tokura, Yoshinori] Univ Tokyo, QPEC, Tokyo 1138656, Japan.
RP Sato, TJ (reprint author), Tohoku Univ, Inst Multidisciplinary Res Adv Mat, 2-1-1 Katahira, Sendai, Miyagi 9808577, Japan.
EM taku@tagen.tohoku.ac.jp
RI Tokura, Yoshinori/C-7352-2009; Okuyama, Daisuke/A-2796-2010; Arima,
Taka-hisa/G-9217-2012; Kikkawa, Akiko/B-3369-2013; Taguchi,
Yasujiro/A-3048-2010; Sato, Taku/I-7664-2015
OI Kikkawa, Akiko/0000-0001-7290-8577; Sato, Taku/0000-0003-2511-4998
FU Japan Society for the Promotion of Science (JSPS) [24224009]; Division
of Scientific User Facilities, Office of Basic Energy Science, U.S.
Department of Energy (DOE); US-Japan Collaborative Program on Neutron
Scattering
FX The authors thank N. Nagaosa, Y. Endoh, and K. Kakurai for stimulating
discussions. This work was partly supported by a Grant-In-Aid for
Scientific Research (24224009) from the Japan Society for the Promotion
of Science (JSPS). The work at HFIR, Oak Ridge National Laboratory, was
sponsored by the Division of Scientific User Facilities, Office of Basic
Energy Science, U.S. Department of Energy (DOE), and was partly
supported by the US-Japan Collaborative Program on Neutron Scattering.
NR 36
TC 0
Z9 0
U1 12
U2 12
PU AMER PHYSICAL SOC
PI COLLEGE PK
PA ONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA
SN 2469-9950
EI 2469-9969
J9 PHYS REV B
JI Phys. Rev. B
PD OCT 19
PY 2016
VL 94
IS 14
AR 144420
DI 10.1103/PhysRevB.94.144420
PG 7
WC Physics, Condensed Matter
SC Physics
GA DZ8BU
UT WOS:000386094400004
ER
PT J
AU Orrigo, SEA
Rubio, B
Gelletly, W
Blank, B
Fujita, Y
Giovinazzo, J
Agramunt, J
Algora, A
Ascher, P
Bilgier, B
Caceres, L
Cakirli, RB
de France, G
Ganioglu, E
Gerbaux, M
Grevy, S
Kamalou, O
Kozer, HC
Kucuk, L
Kurtukian-Nieto, T
Molina, F
Popescu, L
Rogers, AM
Susoy, G
Stodel, C
Suzuki, T
Tamii, A
Thomas, JC
AF Orrigo, S. E. A.
Rubio, B.
Gelletly, W.
Blank, B.
Fujita, Y.
Giovinazzo, J.
Agramunt, J.
Algora, A.
Ascher, P.
Bilgier, B.
Caceres, L.
Cakirli, R. B.
de France, G.
Ganioglu, E.
Gerbaux, M.
Grevy, S.
Kamalou, O.
Kozer, H. C.
Kucuk, L.
Kurtukian-Nieto, T.
Molina, F.
Popescu, L.
Rogers, A. M.
Susoy, G.
Stodel, C.
Suzuki, T.
Tamii, A.
Thomas, J. C.
TI Observation of the 2(+) isomer in Co-52
SO PHYSICAL REVIEW C
LA English
DT Article
ID PROTON-RICH NUCLEI; DECAY; FE-52; BEAM; NUCLEOSYNTHESIS; SPECTROMETER;
REGION; STATES
AB We report the first observation of the 2(+) isomer in Co-52, produced in the beta decay of the 0(+), Ni-52 ground state. We have observed three. rays at 849, 1910, and 5185 keV characterizing the beta de-excitation of the isomer. We have measured a half-life of 102(6) ms for the isomeric state. The Fermi and Gamow-Teller transition strengths for the beta decay of Co-52m to Fe-52 have been determined. We also add new information on the beta decay of the 6(+), Co-52 ground state, for which we have measured a half-life of 112(3) ms.
C1 [Orrigo, S. E. A.; Rubio, B.; Gelletly, W.; Agramunt, J.; Algora, A.; Molina, F.] Univ Valencia, CSIC, Inst Fis Corpuscular, E-46071 Valencia, Spain.
[Gelletly, W.] Univ Surrey, Dept Phys, Guildford GU2 7XH, Surrey, England.
[Blank, B.; Giovinazzo, J.; Ascher, P.; Gerbaux, M.; Grevy, S.; Kurtukian-Nieto, T.] Univ Bordeaux, CNRS IN2P3, Ctr Etud Nucl Bordeaux Gradignan, F-33175 Gradignan, France.
[Fujita, Y.] Osaka Univ, Dept Phys, Toyonaka, Osaka 5600043, Japan.
[Fujita, Y.; Suzuki, T.; Tamii, A.] Osaka Univ, Res Ctr Nucl Phys, Ibaraki, Osaka 5670047, Japan.
[Algora, A.] Hungarian Acad Sci, Inst Nucl Res, H-4026 Debrecen, Hungary.
[Bilgier, B.; Cakirli, R. B.; Kucuk, L.] Istanbul Univ, Dept Phys, TR-34134 Istanbul, Turkey.
[Kamalou, O.; Stodel, C.; Thomas, J. C.] CEA DRF CNRS IN2P3, GANIL, Bvd Henri Becquerel, F-14076 Caen, France.
[Molina, F.] Comis Chilena Energia Nucl, Casilla 188-D, Santiago, Chile.
[Popescu, L.] SCK CEN, Boeretang 200, B-2400 Mol, Belgium.
[Rogers, A. M.] Argonne Natl Lab, Div Phys, Argonne, IL 60439 USA.
RP Orrigo, SEA (reprint author), Univ Valencia, CSIC, Inst Fis Corpuscular, E-46071 Valencia, Spain.
EM sonja.orrigo@ific.uv.es
RI Molina, Francisco/D-5319-2014; Popescu, Lucia/F-9964-2011
OI Molina, Francisco/0000-0002-9459-1336; Popescu,
Lucia/0000-0003-1678-4260
FU Spanish MICINN [FPA2008-06419-C02-01, FPA2011-24553,
FPA2014-52823-C2-1-P]; Centro de Excelencia Severo Ochoa del [IFIC
SEV-2014-0398]; Junta para la Ampliacion de Estudios Programme (CSIC
JAE-Doc contract) - FSE; ENSAR project [262010]; MEXT, Japan [18540270,
22540310]; Japan-Spain collaborative program of JSPS; Japan-Spain
collaborative program of CSIC; UK Science and Technology Facilities
Council (STFC) [ST/F012012/1]; Region of Aquitaine; International Post
Doctoral Research Programme [TUBITAK 2219]; Alexander von Humboldt
foundation; Max-Planck-Partner Group
FX This work was supported by the Spanish MICINN grants no.
FPA2008-06419-C02-01, FPA2011-24553, FPA2014-52823-C2-1-P; Centro de
Excelencia Severo Ochoa del IFIC SEV-2014-0398; Junta para la Ampliacion
de Estudios Programme (CSIC JAE-Doc contract) co-financed by FSE; ENSAR
project no. 262010; MEXT, Japan 18540270 and 22540310; Japan-Spain
collaborative program of JSPS and CSIC; UK Science and Technology
Facilities Council (STFC) Grant No. ST/F012012/1; Region of Aquitaine.
E.G. acknowledges support by TUBITAK 2219 International Post Doctoral
Research Programme. R.B.C. acknowledges support by the Alexander von
Humboldt foundation and the Max-Planck-Partner Group. We acknowledge the
EXOGAM collaboration for the use of their clover detectors.
NR 23
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PU AMER PHYSICAL SOC
PI COLLEGE PK
PA ONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA
SN 2469-9985
EI 2469-9993
J9 PHYS REV C
JI Phys. Rev. C
PD OCT 19
PY 2016
VL 94
IS 4
AR 044315
DI 10.1103/PhysRevC.94.044315
PG 8
WC Physics, Nuclear
SC Physics
GA DZ9CL
UT WOS:000386170700001
ER
PT J
AU Zheng, X
Adhikari, KP
Bosted, P
Deur, A
Drozdov, V
El Fassi, L
Kang, H
Kovacs, K
Kuhn, S
Long, E
Phillips, SK
Ripani, M
Slifer, K
Smith, LC
Adikaram, D
Akbar, Z
Amaryan, MJ
Pereira, SA
Asryan, G
Avakian, H
Badui, RA
Ball, J
Baltzell, NA
Battaglieri, M
Batourine, V
Bedlinskiy, I
Biselli, AS
Briscoe, WJ
Bultmann, S
Burkert, VD
Carman, DS
Celentano, A
Chandavar, S
Charles, G
Chen, JP
Chetry, T
Choi, S
Ciullo, G
Clark, L
Colaneri, L
Cole, PL
Compton, N
Contalbrigo, M
Crede, V
D'Angelo, A
Dashyan, N
De Vita, R
De Sanctis, E
Djalali, C
Dodge, GE
Dupre, R
Egiyan, H
El Alaoui, A
Elouadrhiri, L
Eugenio, P
Fanchini, E
Fedotov, G
Fersch, R
Filippi, A
Fleming, JA
Gevorgyan, N
Ghandilyan, Y
Gilfoyle, GP
Giovanetti, KL
Girod, FX
Gleason, C
Golovach, E
Gothe, RW
Griffioen, KA
Guidal, M
Guler, N
Guo, L
Hanretty, C
Harrison, N
Hattawy, M
Hicks, K
Holtrop, M
Hughes, SM
Ilieva, Y
Ireland, DG
Ishkhanov, BS
Isupov, EL
Jenkins, D
Jiang, H
Jo, HS
Joosten, S
Keller, D
Khachatryan, G
Khandaker, M
Kim, A
Kim, W
Klein, FJ
Kubarovsky, V
Lanza, L
Lenisa, P
Livingston, K
MacGregor, IJD
Markov, N
McKinnon, B
Mirazita, M
Mokeev, V
Movsisyan, A
Munevar, E
Camacho, CM
Murdoch, G
Nadel-Turonski, P
Net, LA
Ni, A
Niccolai, S
Niculescu, G
Niculescu, I
Osipenko, M
Ostrovidov, AI
Paolone, M
Paremuzyan, R
Park, K
Pasyuk, E
Peng, P
Pisano, S
Pogorelko, O
Price, JW
Puckett, AJR
Raue, BA
Rizzo, A
Rosner, G
Rossi, P
Roy, P
Sabatie, F
Salgado, C
Schumacher, RA
Sharabian, YG
Skorodumina, I
Smith, GD
Sokhan, D
Sparveris, N
Stankovic, I
Strakovsky, II
Strauch, S
Taiuti, M
Tian, Y
Ungaro, M
Voskanyan, H
Voutier, E
Walford, NK
Watts, DP
Wei, X
Weinstein, LB
Wood, MH
Zachariou, N
Zhang, J
Zonta, I
AF Zheng, X.
Adhikari, K. P.
Bosted, P.
Deur, A.
Drozdov, V.
El Fassi, L.
Kang, Hyekoo
Kovacs, K.
Kuhn, S.
Long, E.
Phillips, S. K.
Ripani, M.
Slifer, K.
Smith, L. C.
Adikaram, D.
Akbar, Z.
Amaryan, M. J.
Pereira, S. Anefalos
Asryan, G.
Avakian, H.
Badui, R. A.
Ball, J.
Baltzell, N. A.
Battaglieri, M.
Batourine, V.
Bedlinskiy, I.
Biselli, A. S.
Briscoe, W. J.
Bueltmann, S.
Burkert, V. D.
Carman, D. S.
Celentano, A.
Chandavar, S.
Charles, G.
Chen, J. -P.
Chetry, T.
Choi, Seonho
Ciullo, G.
Clark, L.
Colaneri, L.
Cole, P. L.
Compton, N.
Contalbrigo, M.
Crede, V.
D'Angelo, A.
Dashyan, N.
De Vita, R.
De Sanctis, E.
Djalali, C.
Dodge, G. E.
Dupre, R.
Egiyan, H.
El Alaoui, A.
Elouadrhiri, L.
Eugenio, P.
Fanchini, E.
Fedotov, G.
Fersch, R.
Filippi, A.
Fleming, J. A.
Gevorgyan, N.
Ghandilyan, Y.
Gilfoyle, G. P.
Giovanetti, K. L.
Girod, F. X.
Gleason, C.
Golovach, E.
Gothe, R. W.
Griffioen, K. A.
Guidal, M.
Guler, N.
Guo, L.
Hanretty, C.
Harrison, N.
Hattawy, M.
Hicks, K.
Holtrop, M.
Hughes, S. M.
Ilieva, Y.
Ireland, D. G.
Ishkhanov, B. S.
Isupov, E. L.
Jenkins, D.
Jiang, H.
Jo, H. S.
Joosten, S.
Keller, D.
Khachatryan, G.
Khandaker, M.
Kim, A.
Kim, W.
Klein, F. J.
Kubarovsky, V.
Lanza, L.
Lenisa, P.
Livingston, K.
MacGregor, I. J. D.
Markov, N.
McKinnon, B.
Mirazita, M.
Mokeev, V.
Movsisyan, A.
Munevar, E.
Camacho, C. Munoz
Murdoch, G.
Nadel-Turonski, P.
Net, L. A.
Ni, A.
Niccolai, S.
Niculescu, G.
Niculescu, I.
Osipenko, M.
Ostrovidov, A. I.
Paolone, M.
Paremuzyan, R.
Park, K.
Pasyuk, E.
Peng, P.
Pisano, S.
Pogorelko, O.
Price, J. W.
Puckett, A. J. R.
Raue, B. A.
Rizzo, A.
Rosner, G.
Rossi, P.
Roy, P.
Sabatie, F.
Salgado, C.
Schumacher, R. A.
Sharabian, Y. G.
Skorodumina, Iu.
Smith, G. D.
Sokhan, D.
Sparveris, N.
Stankovic, I.
Strakovsky, I. I.
Strauch, S.
Taiuti, M.
Tian, Ye
Ungaro, M.
Voskanyan, H.
Voutier, E.
Walford, N. K.
Watts, D. P.
Wei, X.
Weinstein, L. B.
Wood, M. H.
Zachariou, N.
Zhang, J.
Zonta, I.
CA CLAS Collaboration
TI Measurement of target and double-spin asymmetries for the
(e)over-right-arrow (p)over-right-arrow -> e pi(+)(n) reaction in the
nucleon resonance region at low Q(2)
SO PHYSICAL REVIEW C
LA English
DT Article
AB We report measurements of target- and double-spin asymmetries for the exclusive channel (e) over right arrow (p) over right arrow -> ep(+)(n) in the nucleon resonance region at Jefferson Lab using the CEBAF Large Acceptance Spectrometer (CLAS). These asymmetries were extracted from data obtained using a longitudinally polarized NH3 target and a longitudinally polarized electron beam with energies 1.1, 1.3, 2.0, 2.3, and 3.0 GeV. The new results are consistent with previous CLAS publications but are extended to a low Q(2) range from 0.0065 to 0.35 (GeV/c)(2). The Q(2) access was made possible by a custom-built Cherenkov detector that allowed the detection of electrons for scattering angles as low as 6 degrees. These results are compared with the unitary isobar models JANR and MAID, the partial-wave analysis prediction from SAID, and the dynamic model DMT. In many kinematic regions our results, in particular results on the target asymmetry, help to constrain the polarization-dependent components of these models.
C1 [Zheng, X.; Deur, A.; Kovacs, K.; Smith, L. C.; Hanretty, C.; Keller, D.; Peng, P.] Univ Virginia, Charlottesville, VA 22901 USA.
[Adhikari, K. P.; El Fassi, L.] Mississippi State Univ, Mississippi State, MS 39762 USA.
[Adhikari, K. P.; Kuhn, S.; Adikaram, D.; Amaryan, M. J.; Bueltmann, S.; Dodge, G. E.; Guler, N.; Weinstein, L. B.] Old Dominion Univ, Norfolk, VA 23529 USA.
[Bosted, P.; Deur, A.; Adikaram, D.; Avakian, H.; Baltzell, N. A.; Batourine, V.; Burkert, V. D.; Carman, D. S.; Celentano, A.; Chen, J. -P.; Egiyan, H.; Elouadrhiri, L.; Girod, F. X.; Guo, L.; Hanretty, C.; Harrison, N.; Kubarovsky, V.; Mokeev, V.; Munevar, E.; Nadel-Turonski, P.; Park, K.; Pasyuk, E.; Raue, B. A.; Rossi, P.; Sharabian, Y. G.; Ungaro, M.; Wei, X.; Zhang, J.] Thomas Jefferson Natl Accelerator Facil, Newport News, VA 23606 USA.
[Drozdov, V.; Ripani, M.; Battaglieri, M.; Celentano, A.; De Vita, R.; Fanchini, E.; Osipenko, M.; Taiuti, M.] INFN, Sez Genova, I-16146 Genoa, Italy.
[Drozdov, V.; Fedotov, G.; Golovach, E.; Ishkhanov, B. S.; Isupov, E. L.; Mokeev, V.; Skorodumina, Iu.] Lomonosov Moscow State Univ, Skobeltsyn Inst Nucl Phys, Moscow 119234, Russia.
[El Fassi, L.; Hattawy, M.] Argonne Natl Lab, Argonne, IL 60439 USA.
[Kang, Hyekoo; Choi, Seonho] Seoul Natl Univ, Seoul, South Korea.
[Long, E.; Phillips, S. K.; Slifer, K.; Egiyan, H.; Holtrop, M.; Paremuzyan, R.] Univ New Hampshire, Durham, NH 03824 USA.
[Akbar, Z.; Crede, V.; Eugenio, P.; Ostrovidov, A. I.; Roy, P.] Florida State Univ, Tallahassee, FL 32306 USA.
[Pereira, S. Anefalos; De Sanctis, E.; Mirazita, M.; Pisano, S.; Rossi, P.] INFN, Lab Nazl Frascati, I-00044 Frascati, Italy.
[Asryan, G.; Dashyan, N.; Gevorgyan, N.; Khachatryan, G.; Voskanyan, H.] Yerevan Phys Inst, Yerevan 375036, Armenia.
[Badui, R. A.; Guo, L.; Raue, B. A.] Florida Int Univ, Miami, FL 33199 USA.
[Ball, J.; Girod, F. X.; Sabatie, F.] CEA, Ctr Saclay, Irfu Serv Phys Nucl, F-91191 Gif Sur Yvette, France.
[Baltzell, N. A.; Djalali, C.; Fedotov, G.; Gleason, C.; Gothe, R. W.; Ilieva, Y.; Jiang, H.; Net, L. A.; Skorodumina, Iu.; Strauch, S.; Tian, Ye; Wood, M. H.] Univ S Carolina, Columbia, SC 29208 USA.
[Bedlinskiy, I.; Pogorelko, O.] Inst Theoret & Expt Phys, Moscow 117259, Russia.
[Biselli, A. S.] Fairfield Univ, Fairfield, CT 06824 USA.
[Biselli, A. S.; Schumacher, R. A.] Carnegie Mellon Univ, Pittsburgh, PA 15213 USA.
[Briscoe, W. J.; Ilieva, Y.; Munevar, E.; Strakovsky, I. I.; Strauch, S.] George Washington Univ, Washington, DC 20052 USA.
[Chandavar, S.; Chetry, T.; Compton, N.; Hicks, K.] Ohio Univ, Athens, OH USA.
[Charles, G.; Dupre, R.; Guidal, M.; Jo, H. S.; Camacho, C. Munoz; Niccolai, S.; Voutier, E.] CNRS IN2P3, Inst Phys Nucl, Orsay, France.
[Charles, G.; Dupre, R.; Guidal, M.; Jo, H. S.; Camacho, C. Munoz; Niccolai, S.; Voutier, E.] Univ Paris 11, Orsay, France.
[Ciullo, G.; Contalbrigo, M.; Lenisa, P.; Movsisyan, A.] INFN, Sez Ferrara, I-44100 Ferrara, Italy.
[Clark, L.; Ireland, D. G.; Livingston, K.; MacGregor, I. J. D.; McKinnon, B.; Murdoch, G.; Rosner, G.; Sokhan, D.] Univ Glasgow, Glasgow G12 8QQ, Lanark, Scotland.
[Colaneri, L.; D'Angelo, A.; Lanza, L.; Rizzo, A.; Zonta, I.] INFN, Sez Roma Tor Vergata, I-00133 Rome, Italy.
[Colaneri, L.; D'Angelo, A.; Lanza, L.; Rizzo, A.; Zonta, I.] Univ Roma Tor Vergata, I-00133 Rome, Italy.
[Cole, P. L.; Khandaker, M.] Idaho State Univ, Pocatello, ID 83209 USA.
[El Alaoui, A.] Univ Tecn Federico Santa Maria, Casilla 110-V, Valparaiso, Chile.
[Fersch, R.] Christopher Newport Univ, Newport News, VA 23606 USA.
[Filippi, A.] INFN, Sez Torino, I-10125 Turin, Italy.
[Fleming, J. A.; Hughes, S. M.; Smith, G. D.; Stankovic, I.; Watts, D. P.; Zachariou, N.] Univ Edinburgh, Edinburgh EH9 3JZ, Midlothian, Scotland.
[Gilfoyle, G. P.] Univ Richmond, Richmond, VA 23173 USA.
[Giovanetti, K. L.; Niculescu, G.; Niculescu, I.] James Madison Univ, Harrisonburg, VA 22807 USA.
[Griffioen, K. A.] Coll William & Mary, Williamsburg, VA 23187 USA.
[Jenkins, D.] Virginia Tech, Blacksburg, VA 24061 USA.
[Joosten, S.; Paolone, M.; Sparveris, N.] Temple Univ, Philadelphia, PA 19122 USA.
[Khandaker, M.; Salgado, C.] Norfolk State Univ, Norfolk, VA 23504 USA.
[Kim, A.; Markov, N.; Puckett, A. J. R.; Ungaro, M.] Univ Connecticut, Storrs, CT 06269 USA.
[Kim, W.; Ni, A.; Park, K.] Kyungpook Natl Univ, Daegu 702701, South Korea.
[Klein, F. J.; Nadel-Turonski, P.; Walford, N. K.] Catholic Univ Amer, Washington, DC 20064 USA.
[Kubarovsky, V.] Rensselaer Polytech Inst, Troy, NY 12180 USA.
[Price, J. W.] Calif State Univ Dominguez Hills, Carson, CA 90747 USA.
[Taiuti, M.] Univ Genoa, Dipartimento Fis, I-16146 Genoa, Italy.
[Wood, M. H.] Canisius Coll, Buffalo, NY 14208 USA.
[Guler, N.] Los Alamos Natl Lab, Los Alamos, NM 87544 USA.
RP Hanretty, C (reprint author), Univ Virginia, Charlottesville, VA 22901 USA.; Adikaram, D (reprint author), Old Dominion Univ, Norfolk, VA 23529 USA.; Adikaram, D; Hanretty, C (reprint author), Thomas Jefferson Natl Accelerator Facil, Newport News, VA 23606 USA.
RI Drozdov, Vadim/E-5456-2012; Schumacher, Reinhard/K-6455-2013; D'Angelo,
Annalisa/A-2439-2012; Lanza, Lucilla/E-6479-2017
OI Schumacher, Reinhard/0000-0002-3860-1827; D'Angelo,
Annalisa/0000-0003-3050-4907; Lanza, Lucilla/0000-0002-1280-532X
FU U.S. Department of Energy (DOE); U.S. National Science Foundation; U.S.
Jeffress Memorial Trust; United Kingdom's Science and Technology
Facilities Council (STFC) [ST/L005719/1, GR/T08708/01]; Italian Istituto
Nazionale di Fisica Nucleare; French Institut National de Physique
Nucleaire et de Physique des Particules; French Centre National de la
Recherche Scientifique; National Research Foundation of Korea; U.S.
Department of Energy, Office of Science, Office of Nuclear Physics
[DE-AC05-06OR23177]
FX The authors gratefully acknowledge the work of Jefferson Lab staff in
the Accelerator and Physics Divisions that resulted in the successful
completion of the experiment. This work was supported by the U.S.
Department of Energy (DOE), the U.S. National Science Foundation, the
U.S. Jeffress Memorial Trust, the United Kingdom's Science and
Technology Facilities Council (STFC) under Grants No. ST/L005719/1 and
No. GR/T08708/01, the Italian Istituto Nazionale di Fisica Nucleare, the
French Institut National de Physique Nucleaire et de Physique des
Particules, the French Centre National de la Recherche Scientifique, and
the National Research Foundation of Korea. This material is based upon
work supported by the U.S. Department of Energy, Office of Science,
Office of Nuclear Physics under Contract No. DE-AC05-06OR23177.
NR 54
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PU AMER PHYSICAL SOC
PI COLLEGE PK
PA ONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA
SN 2469-9985
EI 2469-9993
J9 PHYS REV C
JI Phys. Rev. C
PD OCT 19
PY 2016
VL 94
IS 4
AR 045206
DI 10.1103/PhysRevC.94.045206
PG 19
WC Physics, Nuclear
SC Physics
GA DZ9CL
UT WOS:000386170700004
ER
PT J
AU Sudar, N
Musumeci, P
Duris, J
Gadjev, I
Polyanskiy, M
Pogorelsky, I
Fedurin, M
Swinson, C
Kusche, K
Babzien, M
Gover, A
AF Sudar, N.
Musumeci, P.
Duris, J.
Gadjev, I.
Polyanskiy, M.
Pogorelsky, I.
Fedurin, M.
Swinson, C.
Kusche, K.
Babzien, M.
Gover, A.
TI High Efficiency Energy Extraction from a Relativistic Electron Beam in a
Strongly Tapered Undulator
SO PHYSICAL REVIEW LETTERS
LA English
DT Article
ID LASER ACCELERATOR; RADIATION
AB We present results of an experiment where, using a 200 GW CO2 laser seed, a 65 MeV electron beam was decelerated down to 35 MeV in a 54-cm-long strongly tapered helical magnetic undulator, extracting over 30% of the initial electron beam energy to coherent radiation. These results, supported by simulations of the radiation field evolution, demonstrate unparalleled electro-optical conversion efficiencies for a relativistic beam in an undulator field and represent an important step in the development of high peak and average power coherent radiation sources.
C1 [Sudar, N.; Musumeci, P.; Duris, J.; Gadjev, I.] Univ Calif Los Angeles, Dept Phys & Astron, Particle Beam Phys Lab, Los Angeles, CA 90095 USA.
[Polyanskiy, M.; Pogorelsky, I.; Fedurin, M.; Swinson, C.; Kusche, K.; Babzien, M.] Brookhaven Natl Lab, Accelerator Test Facil, Upton, NY 11973 USA.
[Gover, A.] Tel Aviv Univ, Dept Phys Elect, Fac Engn, IL-69978 Tel Aviv, Israel.
RP Sudar, N (reprint author), Univ Calif Los Angeles, Dept Phys & Astron, Particle Beam Phys Lab, Los Angeles, CA 90095 USA.
FU DOE [DE-SC0009914]; U.S. DHS DNDO [2014-DN-077-ARI084-01]; U.S.-Israel
Binational Science Foundation (BSF) Jerusalem, Israel
FX This work was partially supported by DOE Grant No. DE-SC0009914, U.S.
DHS DNDO under Contract No. 2014-DN-077-ARI084-01, and by the
U.S.-Israel Binational Science Foundation (BSF) Jerusalem, Israel. The
authors would also like to thank Gerard Andonian and Ariel Nause for
useful comments.
NR 26
TC 0
Z9 0
U1 1
U2 1
PU AMER PHYSICAL SOC
PI COLLEGE PK
PA ONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA
SN 0031-9007
EI 1079-7114
J9 PHYS REV LETT
JI Phys. Rev. Lett.
PD OCT 19
PY 2016
VL 117
IS 17
AR 174801
DI 10.1103/PhysRevLett.117.174801
PG 5
WC Physics, Multidisciplinary
SC Physics
GA EA1ZY
UT WOS:000386392000004
PM 27824445
ER
PT J
AU Edlund, P
Takala, H
Claesson, E
Henry, L
Dods, R
Lehtivuori, H
Panman, M
Pande, K
White, T
Nakane, T
Berntsson, O
Gustavsson, E
Bath, P
Modi, V
Roy-Chowdhury, S
Zook, J
Berntsen, P
Pandey, S
Poudyal, I
Tenboer, J
Kupitz, C
Barty, A
Fromme, P
Koralek, JD
Tanaka, T
Spence, J
Liang, ML
Hunter, MS
Boutet, S
Nango, E
Moffat, K
Groenhof, G
Ihalainen, J
Stojkovic, EA
Schmidt, M
Westenhoff, S
AF Edlund, Petra
Takala, Heikki
Claesson, Elin
Henry, Leocadie
Dods, Robert
Lehtivuori, Heli
Panman, Matthijs
Pande, Kanupriya
White, Thomas
Nakane, Takanori
Berntsson, Oskar
Gustavsson, Emil
Bath, Petra
Modi, Vaibhav
Roy-Chowdhury, Shatabdi
Zook, James
Berntsen, Peter
Pandey, Suraj
Poudyal, Ishwor
Tenboer, Jason
Kupitz, Christopher
Barty, Anton
Fromme, Petra
Koralek, Jake D.
Tanaka, Tomoyuki
Spence, John
Liang, Mengning
Hunter, Mark S.
Boutet, Sebastien
Nango, Eriko
Moffat, Keith
Groenhof, Gerrit
Ihalainen, Janne
Stojkovic, Emina A.
Schmidt, Marius
Westenhoff, Sebastian
TI The room temperature crystal structure of a bacterial phytochrome
determined by serial femtosecond crystallography
SO SCIENTIFIC REPORTS
LA English
DT Article
ID CHROMOPHORE-BINDING DOMAIN; X-RAY-DIFFRACTION; GROUND-STATE; RED LIGHT;
PROTEIN; BACTERIOPHYTOCHROME; PHOTOCONVERSION; REARRANGEMENTS;
TRANSDUCTION; FLUORESCENCE
AB Phytochromes are a family of photoreceptors that control light responses of plants, fungi and bacteria. A sequence of structural changes, which is not yet fully understood, leads to activation of an output domain. Time-resolved serial femtosecond crystallography (SFX) can potentially shine light on these conformational changes. Here we report the room temperature crystal structure of the chromophore-binding domains of the Deinococcus radiodurans phytochrome at 2.1 angstrom resolution. The structure was obtained by serial femtosecond X-ray crystallography from microcrystals at an X-ray free electron laser. We find overall good agreement compared to a crystal structure at 1.35 angstrom resolution derived from conventional crystallography at cryogenic temperatures, which we also report here. The thioether linkage between chromophore and protein is subject to positional ambiguity at the synchrotron, but is fully resolved with SFX. The study paves the way for time-resolved structural investigations of the phytochrome photocycle with time-resolved SFX.
C1 [Edlund, Petra; Takala, Heikki; Claesson, Elin; Henry, Leocadie; Dods, Robert; Lehtivuori, Heli; Panman, Matthijs; Berntsson, Oskar; Gustavsson, Emil; Bath, Petra; Westenhoff, Sebastian] Univ Gothenburg, Dept Chem & Mol Biol, S-40530 Gothenburg, Sweden.
[Takala, Heikki] Univ Jyvaskyla, Dept Biol & Environm Sci, Jyvaskyla 40014, Finland.
[Takala, Heikki] Univ Helsinki, Fac Med, Anat, FIN-00014 Helsinki, Finland.
[Lehtivuori, Heli] Univ Jyvaskyla, Dept Phys, Nanosci Ctr, Jyvaskyla 40014, Finland.
[Pande, Kanupriya; White, Thomas; Barty, Anton] DESY, Ctr Free Electron Laser Sci, D-22603 Hamburg, Germany.
[Nakane, Takanori] Univ Tokyo, Grad Sch Sci, Dept Biol Sci, Bunkyo Ku, 7-3-1 Hongo, Tokyo 1130033, Japan.
[Modi, Vaibhav; Groenhof, Gerrit] Univ Jyvaskyla, Dept Chem, Nanosci Ctr, Jyvaskyla 40014, Finland.
[Roy-Chowdhury, Shatabdi; Zook, James; Fromme, Petra] Arizona State Univ, Sch Mol Sci, Tempe, AZ 85287 USA.
[Berntsen, Peter] La Trobe Univ, Ctr Excellence Adv Mol Imaging, Australian Res Council, La Trobe Inst Mol Sci, Melbourne, Vic 3086, Australia.
[Pandey, Suraj; Poudyal, Ishwor; Tenboer, Jason; Kupitz, Christopher; Schmidt, Marius] Univ Wisconsin, Dept Phys, Milwaukee, WI 53211 USA.
[Koralek, Jake D.; Liang, Mengning; Hunter, Mark S.; Boutet, Sebastien] SLAC Natl Accelerator Lab, Linac Coherent Light Source, 2575 Sand Hill Rd, Menlo Pk, CA 94025 USA.
[Nango, Eriko] RIKEN SPring 8 Ctr, 1-1-1 Kouto, Sayo, Hyogo 6795148, Japan.
[Spence, John] Arizona State Univ, Biodesign Inst, Tempe, AZ 85287 USA.
[Spence, John] Arizona State Univ, Ctr Appl Struct Discovery, Tempe, AZ 85287 USA.
[Spence, John] Arizona State Univ, Dept Phys, Tempe, AZ 85287 USA.
[Moffat, Keith] Univ Chicago, Dept Biochem & Mol Biol, 920 E 58Th St, Chicago, IL 60637 USA.
[Moffat, Keith] Argonne Natl Lab, BioCARS, Argonne, IL 60439 USA.
[Ihalainen, Janne] Univ Jyvaskyla, Dept Biol & Environm Sci, Nanosci Ctr, Jyvaskyla 40014, Finland.
[Stojkovic, Emina A.] NE Illinois Univ, Dept Biol, 5500 North St Louis Ave, Chicago, IL 60625 USA.
RP Westenhoff, S (reprint author), Univ Gothenburg, Dept Chem & Mol Biol, S-40530 Gothenburg, Sweden.; Schmidt, M (reprint author), Univ Wisconsin, Dept Phys, Milwaukee, WI 53211 USA.
EM smarius@uwm.edu; westenho@chem.gu.se
OI Takala, Heikki/0000-0003-2518-8583; Groenhof, Gerrit/0000-0001-8148-5334
FU European Research Council; Foundation of Strategic Research, Sweden;
National Science Foundation (NSF) MCB grant [1413360]; Academy of
Finland; Finnish Cultural Foundation; Foundation of International
Cooperation in Research and Higher Education, Sweden (STINT); X-ray Free
Electron Laser Priority Strategy Program (MEXT, Japan); U.S. Department
of Energy, Office of Science, Office of Basic Energy Sciences
[DE-AC02-76SF00515]; NIH [P41GM103393]; CFEL DESY through
program-oriented funds of the Helmholtz Association
FX SW acknowledges funding from the European Research Council and the
Foundation of Strategic Research, Sweden. EAS acknowledges funding from
National Science Foundation (NSF) MCB grant 1413360. JAI, HT and HL
acknowledge funding from Academy of Finland and Finnish Cultural
Foundation and the support in protein production provided by Tampere
Protein Technologies Core Facility (V. Hytonen and J. Maatta) under
Biocenter Finland network. SW, GG, and JI acknowledge support by the
Foundation of International Cooperation in Research and Higher
Education, Sweden (STINT). EN, TN, and TT acknowledge support by X-ray
Free Electron Laser Priority Strategy Program (MEXT, Japan) and
computing supports from SACLA HPC and Mini-K. Part of the experiments
were carried out at the BL3 of SACLA with the approval of the Japan
Synchrotron Radiation Research Institute (JASRI) (proposal no.
2014B8050). JCHS, PF and MS acknowledge NSF STC 1231306. Portions of
this research were carried out at the Linac Coherent Light Source (LCLS)
at the SLAC National Accelerator Laboratory. Use of the LCLS, is
supported by the U.S. Department of Energy, Office of Science, Office of
Basic Energy Sciences under Contract No. DE-AC02-76SF00515 Parts of the
sample delivery system used at LCLS for this research was funded by the
NIH grant P41GM103393, formerly P41RR001209. TW, AB, and KP acknowledge
financial support from CFEL DESY through program-oriented funds of the
Helmholtz Association.
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PU NATURE PUBLISHING GROUP
PI LONDON
PA MACMILLAN BUILDING, 4 CRINAN ST, LONDON N1 9XW, ENGLAND
SN 2045-2322
J9 SCI REP-UK
JI Sci Rep
PD OCT 19
PY 2016
VL 6
AR 35279
DI 10.1038/srep35279
PG 9
WC Multidisciplinary Sciences
SC Science & Technology - Other Topics
GA DZ8TX
UT WOS:000386145700001
PM 27756898
ER
PT J
AU Li, QH
Qiao, RM
Wray, LA
Chen, J
Zhuo, ZQ
Chen, YX
Yan, SS
Pan, F
Hussain, Z
Yang, WL
AF Li, Qinghao
Qiao, Ruimin
Wray, L. Andrew
Chen, Jun
Zhuo, Zengqing
Chen, Yanxue
Yan, Shishen
Pan, Feng
Hussain, Zahid
Yang, Wanli
TI Quantitative probe of the transition metal redox in battery electrodes
through soft x-ray absorption spectroscopy
SO JOURNAL OF PHYSICS D-APPLIED PHYSICS
LA English
DT Review
DE soft x-ray absorption spectroscopy; transition-metal redox; Li-ion
batteries; Na-ion batteries
ID LITHIUM-ION BATTERIES; CATHODE MATERIALS; IN-SITU; LINI0.5MN1.5O4
ELECTRODES; LIFEPO4; LITHIATION; EVOLUTION; PHASE; INTERCALATION;
DEPOSITION
AB Most battery positive electrodes operate with a 3d transition-metal (TM) reaction centre. A direct and quantitative probe of the TM states upon electrochemical cycling is valuable for understanding the detailed cycling mechanism and charge diffusion in the electrodes, which is related with many practical parameters of a battery. This review includes a comprehensive summary of our recent demonstrations of five different types of quantitative analysis of the TM states in battery electrodes based on soft x-ray absorption spectroscopy and multiplet calculations. In LiFePO4, a system of a well-known two-phase transformation type, the TM redox could be strictly determined through a simple linear combination of the two end-members. In Mn-based compounds, the Mn states could also be quantitatively evaluated, but a set of reference spectra with all the three possible Mn valences needs to be deliberately selected and considered in the fitting. Although the fluorescence signals suffer the self-absorption distortion, the multiplet calculations could consider the distortion effect, which allows a quantitative determination of the overall Ni oxidation state in the bulk. With the aid of multiplet calculations, one could also achieve a quasi-quantitative analysis of the Co redox evolution in LiCoO2 based on the energy position of the spectroscopic peak. The benefit of multiplet calculations is more important for studying electrode materials with TMs of mixed spin states, as exemplified by the quantitative analysis of the mixed spin Na2-xFe2(CN)(6) system. At the end, we showcase that such quantitative analysis could provide valuable information for optimizing the electrochemical performance of Na0.44MnO2 electrodes for Na-ion batteries. The methodology summarized in this review could be extended to other energy application systems with TM redox centre for detailed analysis, for example, fuel cell and catalytic materials.
C1 [Li, Qinghao; Chen, Jun; Chen, Yanxue; Yan, Shishen] Shandong Univ, Sch Phys, Natl Key Lab Crystal Mat, Jinan 250100, Peoples R China.
[Li, Qinghao; Qiao, Ruimin; Zhuo, Zengqing; Hussain, Zahid; Yang, Wanli] Lawrence Berkeley Natl Lab, Adv Light Source, Berkeley, CA 94720 USA.
[Wray, L. Andrew] NYU, Dept Phys, 4 Washington Pl, New York, NY 10003 USA.
[Zhuo, Zengqing; Pan, Feng] Peking Univ, Sch Adv Mat, Shenzhen Grad Sch, Shenzhen 518055, Peoples R China.
RP Yan, SS (reprint author), Shandong Univ, Sch Phys, Natl Key Lab Crystal Mat, Jinan 250100, Peoples R China.
EM shishenyan@sdu.edu.cn; wlyang@lbl.gov
RI Yang, Wanli/D-7183-2011; Qiao, Ruimin/E-9023-2013
OI Yang, Wanli/0000-0003-0666-8063;
FU NSFC [11434006]; 111 project [B13029]; Office of Science, Office of
Basic Energy Sciences, of the U.S. Department of Energy
[DE-AC02-05CH11231]; MRSEC Program of the National Science Foundation
[DMR-1420073]; China Scholarship Council (CSC)
FX This work is supported by the key program of NSFC No. 11434006, and the
111 project No. B13029. sXAS data were collected at beamline 8.0.1 of
the Advanced Light Source, which is supported by the Director, Office of
Science, Office of Basic Energy Sciences, of the U.S. Department of
Energy under Contract No. DE-AC02-05CH11231. The calculation works are
supported by the MRSEC Program of the National Science Foundation under
Award Number DMR-1420073. QL thanks the financial support from the China
Scholarship Council (CSC).
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PU IOP PUBLISHING LTD
PI BRISTOL
PA TEMPLE CIRCUS, TEMPLE WAY, BRISTOL BS1 6BE, ENGLAND
SN 0022-3727
EI 1361-6463
J9 J PHYS D APPL PHYS
JI J. Phys. D-Appl. Phys.
PD OCT 19
PY 2016
VL 49
IS 41
AR 413003
DI 10.1088/0022-3727/49/41/413003
PG 14
WC Physics, Applied
SC Physics
GA DY8LZ
UT WOS:000385383000003
ER
PT J
AU Oh, J
Le, MD
Nahm, HH
Sim, H
Jeong, J
Perring, TG
Woo, H
Nakajima, K
Ohira-Kawamura, S
Yamani, Z
Yoshida, Y
Eisaki, H
Cheong, SW
Chernyshev, AL
Park, JG
AF Oh, Joosung
Le, Manh Duc
Nahm, Ho-Hyun
Sim, Hasung
Jeong, Jaehong
Perring, T. G.
Woo, Hyungje
Nakajima, Kenji
Ohira-Kawamura, Seiko
Yamani, Zahra
Yoshida, Y.
Eisaki, H.
Cheong, S. -W.
Chernyshev, A. L.
Park, Je-Geun
TI Spontaneous decays of magneto-elastic excitations in non-collinear
antiferromagnet (Y,Lu)MnO3
SO NATURE COMMUNICATIONS
LA English
DT Article
ID MAGNON-PHONON INTERACTION; MANGANITES; WAVES
AB Magnons and phonons are fundamental quasiparticles in a solid and can be coupled together to form a hybrid quasi-particle. However, detailed experimental studies on the underlying Hamiltonian of this particle are rare for actual materials. Moreover, the anharmonicity of such magnetoelastic excitations remains largely unexplored, although it is essential for a proper understanding of their diverse thermodynamic behaviour and intrinsic zero-temperature decay. Here we show that in non-collinear antiferromagnets, a strong magnon-phonon coupling can significantly enhance the anharmonicity, resulting in the creation of magnetoelastic excitations and their spontaneous decay. By measuring the spin waves over the full Brillouin zone and carrying out anharmonic spin wave calculations using a Hamiltonian with an explicit magnon-phonon coupling, we have identified a hybrid magnetoelastic mode in (Y,Lu)MnO3 and quantified its decay rate and the exchange-striction coupling term required to produce it.
C1 [Oh, Joosung; Le, Manh Duc; Nahm, Ho-Hyun; Sim, Hasung; Jeong, Jaehong; Park, Je-Geun] Ctr Correlated Electron Syst, Inst Basic Sci, Seoul 08826, South Korea.
[Oh, Joosung; Le, Manh Duc; Nahm, Ho-Hyun; Sim, Hasung; Jeong, Jaehong; Park, Je-Geun] Seoul Natl Univ, Dept Phys & Astron, Seoul 08826, South Korea.
[Perring, T. G.; Woo, Hyungje] STFC Rutherford Appleton Lab, ISIS Facil, Didcot OX11 0QX, Oxon, England.
[Woo, Hyungje] Brookhaven Natl Lab, Dept Phys, Upton, NY 11973 USA.
[Nakajima, Kenji; Ohira-Kawamura, Seiko] Japan Atom Energy Agcy, J PARC Ctr, Mat & Life Sci Div, Tokai, Ibaraki 3191195, Japan.
[Yamani, Zahra] CNR, Chalk River Labs, Chalk River, ON K0J 1J0, Canada.
[Yoshida, Y.; Eisaki, H.] Natl Inst Adv Ind Sci & Technol, Tsukuba, Ibaraki 3058565, Japan.
[Cheong, S. -W.] Rutgers State Univ, Dept Phys & Astron, Piscataway, NJ 08854 USA.
[Cheong, S. -W.] Rutgers State Univ, Rutgers Ctr Emergent Mat, Piscataway, NJ 08854 USA.
[Chernyshev, A. L.] Univ Calif Irvine, Dept Phys & Astron, Irvine, CA 92697 USA.
RP Park, JG (reprint author), Ctr Correlated Electron Syst, Inst Basic Sci, Seoul 08826, South Korea.; Park, JG (reprint author), Seoul Natl Univ, Dept Phys & Astron, Seoul 08826, South Korea.
EM jgpark10@snu.ac.kr
RI Park, Je Geun/K-8571-2013;
OI Le, Manh Duc/0000-0003-3012-6053
FU Institute for Basic Science [IBS-R009-G1]; U.S. DOE, Office of Science,
Basic Energy Sciences [DE-FG02-04ER46174]; DOE [DOE: DE-FG02-07ER46382]
FX We thank Kisoo Park and W.J.L. Buyers for useful discussions. The work
at the IBS CCES was supported by the research programme of Institute for
Basic Science (IBS-R009-G1). Experiment at J-PARC was carried out
through the proposal number (2011B0064). The work of ALC was supported
by the U.S. DOE, Office of Science, Basic Energy Sciences under Award
Number DE-FG02-04ER46174. The work at Rutgers University was supported
by the DOE under Grant Number DOE: DE-FG02-07ER46382.
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PU NATURE PUBLISHING GROUP
PI LONDON
PA MACMILLAN BUILDING, 4 CRINAN ST, LONDON N1 9XW, ENGLAND
SN 2041-1723
J9 NAT COMMUN
JI Nat. Commun.
PD OCT 19
PY 2016
VL 7
AR 13146
DI 10.1038/ncomms13146
PG 6
WC Multidisciplinary Sciences
SC Science & Technology - Other Topics
GA DZ1RR
UT WOS:000385617400001
PM 27759004
ER
PT J
AU Ryu, WH
Gittleson, FS
Thomsen, JM
Li, JY
Schwab, MJ
Brudvig, GW
Taylor, AD
AF Ryu, Won-Hee
Gittleson, Forrest S.
Thomsen, Julianne M.
Li, Jinyang
Schwab, Mark J.
Brudvig, Gary W.
Taylor, Andre D.
TI Heme biomolecule as redox mediator and oxygen shuttle for efficient
charging of lithium-oxygen batteries
SO NATURE COMMUNICATIONS
LA English
DT Article
ID LI-O-2 BATTERIES; AIR BATTERIES; CATALYST; CHALLENGES; OXIDATION;
MYOGLOBIN; RECHARGEABILITY; ARCHITECTURE; PERFORMANCE; HEMOGLOBIN
AB One of the greatest challenges with lithium-oxygen batteries involves identifying catalysts that facilitate the growth and evolution of cathode species on an oxygen electrode. Heterogeneous solid catalysts cannot adequately address the problematic overpotentials when the surfaces become passivated. However, there exists a class of biomolecules which have been designed by nature to guide complex solution-based oxygen chemistries. Here, we show that the heme molecule, a common porphyrin cofactor in blood, can function as a soluble redox catalyst and oxygen shuttle for efficient oxygen evolution in non-aqueous Li-O-2 batteries. The heme's oxygen binding capability facilitates battery recharge by accepting and releasing dissociated oxygen species while benefiting charge transfer with the cathode. We reveal the chemical change of heme redox molecules where synergy exists with the electrolyte species. This study brings focus to the rational design of solution-based catalysts and suggests a sustainable cross-link between biomolecules and advanced energy storage.
C1 [Ryu, Won-Hee; Gittleson, Forrest S.; Li, Jinyang; Schwab, Mark J.; Taylor, Andre D.] Yale Univ, Dept Chem & Environm Engn, 9 Hillhouse Ave, New Haven, CT 06520 USA.
[Ryu, Won-Hee] Sookmyung Womens Univ, Dept Chem & Biol Engn, 100 Cheongpa Ro 47 Gil, Seoul, South Korea.
[Ryu, Won-Hee] Nature Conservancy, 1815 N Lynn St, Arlington, VA USA.
[Gittleson, Forrest S.] Sandia Natl Labs, Dept Chem Mat, 7011 East Ave, Livermore, CA 94550 USA.
[Thomsen, Julianne M.; Brudvig, Gary W.] Yale Univ, Dept Chem, 225 Prospect St, New Haven, CT USA.
RP Taylor, AD (reprint author), Yale Univ, Dept Chem & Environm Engn, 9 Hillhouse Ave, New Haven, CT 06520 USA.
EM andre.taylor@yale.edu
FU NatureNet Program of the Nature Conservancy; NSF [MRSEC DMR 1119826];
Department of Energy, Office of Basic Energy Sciences, Divisions of
Chemical Sciences [DE-FG02-07ER15909]; U.S. DOE Office of Science User
Facility at Brookhaven National Laboratory [DE-SC0012704]; Basic Science
Research Program through the National Research Foundation of Korea (NRF)
- Ministry of Science, ICT & Future Planning [2016R1C1B2011442];
Sookmyung Women's University Research Grants [1-1603-2014]; U.S.
Department of Energy's National Nuclear Security Administration
[DE-AC04-94AL85000]; [NSF-CBET-0954985 PECASE]
FX We gratefully acknowledge Dr Lisa Pfefferle for the use of Raman
equipment and Dr Menachem Elimelech for the use of the ultraviolet-vis
spectrophotometer and Dr Xiao Tong for assistance with XPS measurements.
W-H.R. acknowledges support from The NatureNet Program of the Nature
Conservancy. We are grateful for the support from NSF under Grant MRSEC
DMR 1119826 (CRISP) and A.D.T acknowledges NSF-CBET-0954985 PECASE Award
for providing partial support of this work. Electrochemical and
ultraviolet-vis spectroscopic studies were supported by a grant from the
Department of Energy, Office of Basic Energy Sciences, Divisions of
Chemical Sciences (DE-FG02-07ER15909 to G.W.B.). The Yale Institute for
Nanoscience and Quantum Engineering (YINQE) and NSF MRSEC DMR 1119826
(CRISP) provided facility support. This research used resources of the
Centre for Functional Nanomaterials, which is a U.S. DOE Office of
Science User Facility, at Brookhaven National Laboratory under Contract
No. DE-SC0012704. This research was supported by Basic Science Research
Program through the National Research Foundation of Korea (NRF) funded
by the Ministry of Science, ICT & Future Planning (2016R1C1B2011442).
This Research was supported by the Sookmyung Women's University Research
Grants 1-1603-2014. Chasm Technologies are acknowledged for their kind
supply of multi-walled carbon nanotubes. Sandia National Laboratories is
a multiprogram laboratory managed and operated by Sandia Corporation, a
wholly owned subsidiary of Lockheed Martin Corporation, for the U.S.
Department of Energy's National Nuclear Security Administration under
contract DE-AC04-94AL85000.
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PI LONDON
PA MACMILLAN BUILDING, 4 CRINAN ST, LONDON N1 9XW, ENGLAND
SN 2041-1723
J9 NAT COMMUN
JI Nat. Commun.
PD OCT 19
PY 2016
VL 7
AR 12925
DI 10.1038/ncomms12925
PG 10
WC Multidisciplinary Sciences
SC Science & Technology - Other Topics
GA DZ1RP
UT WOS:000385617200001
PM 27759005
ER
PT J
AU Wang, ZJ
Dong, JC
Cui, Y
Eres, G
Timpe, O
Fu, Q
Ding, F
Schloegl, R
Willinger, MG
AF Wang, Zhu-Jun
Dong, Jichen
Cui, Yi
Eres, Gyula
Timpe, Olaf
Fu, Qiang
Ding, Feng
Schloegl, R.
Willinger, Marc-Georg
TI Stacking sequence and interlayer coupling in few-layer graphene revealed
by in situ imaging
SO NATURE COMMUNICATIONS
LA English
DT Article
ID CHEMICAL-VAPOR-DEPOSITION; NI ALLOY FOILS; BILAYER GRAPHENE; EPITAXIAL
GRAPHENE; GROWTH; EDGE; CU; GRAPHITE; KINETICS; ENERGY
AB In the transition from graphene to graphite, the addition of each individual graphene layer modifies the electronic structure and produces a different material with unique properties. Controlled growth of few-layer graphene is therefore of fundamental interest and will provide access to materials with engineered electronic structure. Here we combine isothermal growth and etching experiments with in situ scanning electron microscopy to reveal the stacking sequence and interlayer coupling strength in few-layer graphene. The observed layer-dependent etching rates reveal the relative strength of the graphene-graphene and graphene-substrate interaction and the resulting mode of adlayer growth. Scanning tunnelling microscopy and density functional theory calculations confirm a strong coupling between graphene edge atoms and platinum. Simulated etching confirms that etching can be viewed as reversed growth. This work demonstrates that real-time imaging under controlled atmosphere is a powerful method for designing synthesis protocols for sp(2) carbon nanostructures in between graphene and graphite.
C1 [Wang, Zhu-Jun; Timpe, Olaf; Schloegl, R.; Willinger, Marc-Georg] Max Planck Gesell, Fritz Haber Inst, Dept Inorgan Chem, D-14195 Berlin, Germany.
[Dong, Jichen; Ding, Feng] Hong Kong Polytech Univ, Inst Text & Clothing, Hong Kong 999077, Hong Kong, Peoples R China.
[Cui, Yi] Chinese Acad Sci, Suzhou Inst Nano Tech & Nano Bion, 3Vacuum Interconnected Nanotech Workstn, Suzhou 215123, Peoples R China.
[Eres, Gyula] Oak Ridge Natl Lab, Div Mat Sci & Technol, Oak Ridge, TN 37831 USA.
[Fu, Qiang] Chinese Acad Sci, Dalian Inst Chem Phys, State Key Lab Catalysis, Dalian 116023, Peoples R China.
RP Willinger, MG (reprint author), Max Planck Gesell, Fritz Haber Inst, Dept Inorgan Chem, D-14195 Berlin, Germany.
EM willinger@fhi-berlin.mpg.de
RI Ding, Feng/D-5938-2011; Eres, Gyula/C-4656-2017;
OI Ding, Feng/0000-0001-9153-9279; Eres, Gyula/0000-0003-2690-5214; Fu,
Qiang/0000-0001-5316-6758
FU National Science Foundation of China [21573186, 21273189]; U.S.
Department of Energy (DOE), Office of Science (OS), Basic Energy
Sciences (BES), Materials Sciences and Engineering Division; NANO-X
Workstation in Suzhou; Thousand Young Talents Program in China
FX The work done in Hong Kong PolyU was supported by National Science
Foundation of China (21573186 and 21273189). The contribution to this
work by G.E. was supported by the U.S. Department of Energy (DOE),
Office of Science (OS), Basic Energy Sciences (BES), Materials Sciences
and Engineering Division. Y.C. is grateful for support from the NANO-X
Workstation in Suzhou and Thousand Young Talents Program in China.
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PI LONDON
PA MACMILLAN BUILDING, 4 CRINAN ST, LONDON N1 9XW, ENGLAND
SN 2041-1723
J9 NAT COMMUN
JI Nat. Commun.
PD OCT 19
PY 2016
VL 7
AR 13256
DI 10.1038/ncomms13256
PG 12
WC Multidisciplinary Sciences
SC Science & Technology - Other Topics
GA DZ1RX
UT WOS:000385618100002
PM 27759024
ER
PT J
AU Xie, HM
Ben-Zvi, I
Rao, T
Xin, TM
Wang, ED
AF Xie, Huamu
Ben-Zvi, Ilan
Rao, Triveni
Xin, Tianmu
Wang, Erdong
TI Experimental measurements and theoretical model of the cryogenic
performance of bialkali photocathode and characterization with Monte
Carlo simulation
SO PHYSICAL REVIEW ACCELERATORS AND BEAMS
LA English
DT Article
ID TEMPERATURE-DEPENDENCE; ENERGY-GAP; GAAS; SEMICONDUCTORS
AB High-average-current, high-brightness electron sources have important applications, such as in high-repetition- rate free-electron lasers, or in the electron cooling of hadrons. Bialkali photocathodes are promising high-quantum-efficiency (QE) cathode materials, while superconducting rf (SRF) electron guns offer continuous-mode operation at high acceleration, as is needed for high-brightness electron sources. Thus, we must have a comprehensive understanding of the performance of bialkali photocathode at cryogenic temperatures when they are to be used in SRF guns. To remove the heat produced by the radio-frequency field in these guns, the cathode should be cooled to cryogenic temperatures. We recorded an 80% reduction of the QE upon cooling the K2CsSb cathode from room temperature down to the temperature of liquid nitrogen in Brookhaven National Laboratory (BNL)' s 704 MHz SRF gun. We conducted several experiments to identify the underlying mechanism in this reduction. The change in the spectral response of the bialkali photocathode, when cooled from room temperature (300 K) to 166 K, suggests that a change in the ionization energy (defined as the energy gap from the top of the valence band to vacuum level) is the main reason for this reduction. We developed an analytical model of the process, based on Spicer's three-step model. The change in ionization energy, with falling temperature, gives a simplified description of the QE's temperature dependence. We also developed a 2D Monte Carlo code to simulate photoemission that accounts for the wavelength-dependent photon absorption in the first step, the scattering and diffusion in the second step, and the momentum conservation in the emission step. From this simulation, we established a correlation between ionization energy and reduction in the QE. The simulation yielded results comparable to those from the analytical model. The simulation offers us additional capabilities such as calculation of the intrinsic emittance, the temporal response, and the thickness dependence of the QE for the K2CsSb photocathode.
C1 [Xie, Huamu] Peking Univ, Inst Heavy Ion Phys, State Key Lab Nucl Phys & Technol, Beijing 100871, Peoples R China.
[Ben-Zvi, Ilan; Rao, Triveni; Xin, Tianmu; Wang, Erdong] Brookhaven Natl Lab, Upton, NY 11973 USA.
[Ben-Zvi, Ilan] SUNY Stony Brook, Stony Brook, NY 11794 USA.
RP Wang, ED (reprint author), Brookhaven Natl Lab, Upton, NY 11973 USA.
EM wange@bnl.gov
FU Brookhaven Science Associates, LLC [DE-SC0012704]; U.S. Department of
Energy
FX This work was supported by Brookhaven Science Associates, LLC under
Contract No. DE-SC0012704 with the U.S. Department of Energy. We would
like to thank Dr. John Smedley for useful discussions on photoemission
physics. We appreciate the useful discussions we had with Dr. Dimitre
Dimitrov on developing the photoemission code. We appreciate the
cooperation of the research group working on the ERL SRF gun who allowed
us to be involved in testing our cathode in the 704 MHz gun.
NR 26
TC 0
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U1 7
U2 7
PU AMER PHYSICAL SOC
PI COLLEGE PK
PA ONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA
SN 2469-9888
J9 PHYS REV ACCEL BEAMS
JI Phys. Rev. Accel. Beams
PD OCT 19
PY 2016
VL 19
IS 10
AR 103401
DI 10.1103/PhysRevAccelBeams.19.103401
PG 12
WC Physics, Nuclear; Physics, Particles & Fields
SC Physics
GA DZ6NB
UT WOS:000385978100001
ER
PT J
AU Ward, DR
Kim, D
Savage, DE
Lagally, MG
Foote, RH
Friesen, M
Coppersmith, SN
Eriksson, MA
AF Ward, Daniel R.
Kim, Dohun
Savage, Donald E.
Lagally, Max G.
Foote, Ryan H.
Friesen, Mark
Coppersmith, Susan N.
Eriksson, Mark A.
TI State-conditional coherent charge qubit oscillations in a Si/SiGe
quadruple quantum dot
SO NPJ QUANTUM INFORMATION
LA English
DT Article
ID SINGLE-ELECTRON SPIN; SILICON; TOMOGRAPHY
AB Universal quantum computation requires high-fidelity single-qubit rotations and controlled two-qubit gates. Along with high-fidelity single-qubit gates, strong efforts have been made in developing robust two-qubit logic gates in electrically gated quantum dot systems to realise a compact and nanofabrication-compatible architecture. Here we perform measurements of state-conditional coherent oscillations of a charge qubit. Using a quadruple quantum dot formed in a Si/SiGe heterostructure, we show the first demonstration of coherent two-axis control of a double quantum dot charge qubit in undoped Si/SiGe, performing Larmor and Ramsey oscillation measurements. We extract the strength of the capacitive coupling between a pair of double quantum dots by measuring the detuning energy shift (approximate to 75 mu eV) of one double dot depending on the excess charge configuration of the other double dot. We further demonstrate that the strong capacitive coupling allows fast, state-conditional Landau-Zener-Stckelberg oscillations with a conditional pi phase flip time of about 80 ps, showing a promising pathway towards multi-qubit entanglement and control in semiconductor quantum dots.
C1 [Ward, Daniel R.; Kim, Dohun; Foote, Ryan H.; Friesen, Mark; Coppersmith, Susan N.; Eriksson, Mark A.] Univ Wisconsin, Dept Phys, 1150 Univ Ave, Madison, WI 53706 USA.
[Ward, Daniel R.] Sandia Natl Labs, POB 5800, Albuquerque, NM 87185 USA.
[Kim, Dohun] Seoul Natl Univ, Dept Phys & Astron, Seoul, South Korea.
[Savage, Donald E.; Lagally, Max G.] Univ Wisconsin, Dept Mat Sci & Engn, 1509 Univ Ave, Madison, WI 53706 USA.
RP Eriksson, MA (reprint author), Univ Wisconsin, Dept Phys, 1150 Univ Ave, Madison, WI 53706 USA.
EM maeriksson@wisc.edu
FU ARO [W911NF-12-0607]; NSF [DMR-1206915, PHY-1104660]; ONR
[N00014-15-1-0029]; Department of Defense; Korea Institute of Science
and Technology Institutional Program [2E26681]; Laboratory Directed
Research and Development program at Sandia National Laboratories; U.S.
Department of Energy's National Nuclear Security Administration
[DE-AC04-94AL85000]; DOE [DE-FG02-03ER46028]; NSF
FX This work was supported in part by ARO (W911NF-12-0607), NSF
(DMR-1206915, PHY-1104660), ONR (N00014-15-1-0029) and the Department of
Defense. DK acknowledges support from the Korea Institute of Science and
Technology Institutional Program (Project No. 2E26681). The views and
conclusions contained in this document are those of the authors and
should not be interpreted as representing the official policies, either
expressly or implied, of the US Government. Work was also supported by
the Laboratory Directed Research and Development program at Sandia
National Laboratories. Sandia National Laboratories is a multiprogram
laboratory managed and operated by Sandia Corporation, a wholly owned
subsidiary of Lockheed Martin Corporation, for the U.S. Department of
Energy's National Nuclear Security Administration under contract
DE-AC04-94AL85000. Development and maintenance of the growth facilities
used for fabricating samples is supported by DOE (DE-FG02-03ER46028).
This research utilized NSF-supported shared facilities at the University
of Wisconsin-Madison.
NR 50
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U1 5
U2 5
PU NATURE PUBLISHING GROUP
PI LONDON
PA MACMILLAN BUILDING, 4 CRINAN ST, LONDON N1 9XW, ENGLAND
SN 2056-6387
J9 NPJ QUANTUM INFORM
PD OCT 18
PY 2016
VL 2
AR 16032
DI 10.1038/npjqi.2016.32
PG 6
WC Physics, Applied; Physics, Atomic, Molecular & Chemical; Physics,
Condensed Matter
SC Physics
GA EI1YK
UT WOS:000392282600001
ER
PT J
AU Qian, JF
Adams, BD
Zheng, JM
Xu, W
Henderson, WA
Wang, J
Bowden, ME
Xu, SC
Hu, JZ
Zhang, JG
AF Qian, Jiangfeng
Adams, Brian D.
Zheng, Jianming
Xu, Wu
Henderson, Wesley A.
Wang, Jun
Bowden, Mark E.
Xu, Suochang
Hu, Jianzhi
Zhang, Ji-Guang
TI Anode-Free Rechargeable Lithium Metal Batteries
SO ADVANCED FUNCTIONAL MATERIALS
LA English
DT Article
ID ELECTRODEPOSITION; LIQUID; ION
AB Anode-free rechargeable lithium (Li) batteries (AFLBs) are phenomenal energy storage systems due to their significantly increased energy density and reduced cost relative to Li-ion batteries, as well as ease of assembly because of the absence of an active (reactive) anode material. However, significant challenges, including Li dendrite growth and low cycling Coulombic efficiency (CE), have prevented their practical implementation. Here, an anode-free rechargeable lithium battery based on a Cu parallel to LiFePO4 cell structure with an extremely high CE (>99.8%) is reported for the first time. This results from the utilization of both an exceptionally stable electrolyte and optimized charge/discharge protocols, which minimize the corrosion of the in situly formed Li metal anode.
C1 [Qian, Jiangfeng; Adams, Brian D.; Xu, Wu; Hu, Jianzhi; Zhang, Ji-Guang] Pacific Northwest Natl Lab, JCESR, Richland, WA 99354 USA.
[Qian, Jiangfeng; Adams, Brian D.; Zheng, Jianming; Xu, Wu; Henderson, Wesley A.; Zhang, Ji-Guang] Pacific Northwest Natl Lab, Energy & Environm Directorate, Richland, WA 99354 USA.
[Wang, Jun] A123 Syst Res & Dev, Waltham, MA 02451 USA.
[Bowden, Mark E.] Pacific Northwest Natl Lab, Environm & Mol Sci Lab, Richland, WA 99354 USA.
[Xu, Suochang; Hu, Jianzhi] Pacific Northwest Natl Lab, Earth & Biol Sci Directorate, Richland, WA 99354 USA.
RP Zhang, JG (reprint author), Pacific Northwest Natl Lab, JCESR, Richland, WA 99354 USA.; Zhang, JG (reprint author), Pacific Northwest Natl Lab, Energy & Environm Directorate, Richland, WA 99354 USA.
EM jiguang.zhang@pnnl.gov
RI Hu, Jian Zhi/F-7126-2012;
OI Xu, Wu/0000-0002-2685-8684
FU Joint Center for Energy Storage Research, an Energy Innovation Hub -
U.S. Department of Energy (DOE), Office of Science, Basic Energy
Sciences; DOE's Office of Biological and Environmental Research (BER)
FX J.Q. and B.D.A. contributed equally to this work. This work was
supported as part of the Joint Center for Energy Storage Research, an
Energy Innovation Hub funded by the U.S. Department of Energy (DOE),
Office of Science, Basic Energy Sciences. The SEM and XPS
characterizations were conducted in the William R. Wiley Environmental
Molecular Sciences Laboratory (EMSL)-a national scientific user facility
located at Pacific Northwest National Laboratory which is sponsored by
the DOE's Office of Biological and Environmental Research (BER). The
authors would also like to thank Ronnie Wilkins for preparing the LFP
electrodes. J.-G.Z., J.Q. and B.D.A. conceived of the idea and designed
the experiments with assistance from J.Z., W.X., and W.A.H. J.Q. and
B.D.A. prepared the samples and performed the electrochemical and SEM
measurements. J.W. designed the LiFePO4 electrodes. M.E.B.
performed the XPS measurements. S.C. Xu and J. Hu contributed the NMR
results. J.Q., B.D.A., W.A.H., and J.-G.Z. prepared the paper with input
from other authors. The authors declare no competing financial interest.
NR 24
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U1 82
U2 82
PU WILEY-V C H VERLAG GMBH
PI WEINHEIM
PA POSTFACH 101161, 69451 WEINHEIM, GERMANY
SN 1616-301X
EI 1616-3028
J9 ADV FUNCT MATER
JI Adv. Funct. Mater.
PD OCT 18
PY 2016
VL 26
IS 39
BP 7094
EP 7102
DI 10.1002/adfm.201602353
PG 9
WC Chemistry, Multidisciplinary; Chemistry, Physical; Nanoscience &
Nanotechnology; Materials Science, Multidisciplinary; Physics, Applied;
Physics, Condensed Matter
SC Chemistry; Science & Technology - Other Topics; Materials Science;
Physics
GA EB1VW
UT WOS:000387145300006
ER
PT J
AU Gillett, NP
Shiogama, H
Funke, B
Hegerl, G
Knutti, R
Matthes, K
Santer, BD
Stone, D
Tebaldi, C
AF Gillett, Nathan P.
Shiogama, Hideo
Funke, Bernd
Hegerl, Gabriele
Knutti, Reto
Matthes, Katja
Santer, Benjamin D.
Stone, Daithi
Tebaldi, Claudia
TI The Detection and Attribution Model Intercomparison Project (DAMIP v1.0)
contribution to CMIP6
SO GEOSCIENTIFIC MODEL DEVELOPMENT
LA English
DT Article
ID NEAR-SURFACE TEMPERATURE; CLIMATE SENSITIVITY; EXPERIMENTAL-DESIGN;
UNCERTAINTY; VARIABILITY; ATMOSPHERE; HIATUS; SIMULATIONS; PREDICTIONS;
TRENDS
AB Detection and attribution (D&A) simulations were important components of CMIP5 and underpinned the climate change detection and attribution assessments of the Fifth Assessment Report of the Intergovernmental Panel on Climate Change. The primary goals of the Detection and Attribution Model Intercomparison Project (DAMIP) are to facilitate improved estimation of the contributions of anthropogenic and natural forcing changes to observed global warming as well as to observed global and regional changes in other climate variables; to contribute to the estimation of how historical emissions have altered and are altering contemporary climate risk; and to facilitate improved observationally constrained projections of future climate change. D&A studies typically require unforced control simulations and historical simulations including all major anthropogenic and natural forcings. Such simulations will be carried out as part of the DECK and the CMIP6 historical simulation. In addition D&A studies require simulations covering the historical period driven by individual forcings or subsets of forcings only: such simulations are proposed here. Key novel features of the experimental design presented here include firstly new historical simulations with aerosols-only, stratosphericozone-only, CO2-only, solar-only, and volcanic-only forcing, facilitating an improved estimation of the climate response to individual forcing, secondly future single forcing experiments, allowing observationally constrained projections of future climate change, and thirdly an experimental design which allows models with and without coupled atmospheric chemistry to be compared on an equal footing.
C1 [Gillett, Nathan P.] Univ Victoria, Environm & Climate Change Canada, Canadian Ctr Climate Modelling & Anal, Victoria, BC V8W 2Y2, Canada.
[Shiogama, Hideo] Natl Inst Environm Studies, Ctr Global Environm Res, Tsukuba, Ibaraki 3058506, Japan.
[Funke, Bernd] CSIC, Inst Astrofis Andalucia, Glorieta Astron S-N, Granada 18008, Spain.
[Hegerl, Gabriele] Univ Edinburgh, Sch GeoSci, James Hutton Rd, Edinburgh EH9 3FE, Midlothian, Scotland.
[Knutti, Reto] ETH, Inst Atmospher & Climate Sci, Univ Str 16, CH-8092 Zurich, Switzerland.
[Matthes, Katja] GEOMAR Helmholtz Ctr Ocean Res Kiel, Ocean Circulat & Climate Dynam, D-24105 Kiel, Germany.
[Matthes, Katja] Univ Kiel, D-24105 Kiel, Germany.
[Santer, Benjamin D.] Lawrence Livermore Natl Lab, Program Climate Model Diag & Intercomparison, Livermore, CA 94550 USA.
[Stone, Daithi] Lawrence Berkeley Natl Lab, Computat Chem Mat & Climate, Berkeley, CA 94720 USA.
[Tebaldi, Claudia] Natl Ctr Atmospher Res, Climate & Global Dynam Lab, Boulder, CO 80305 USA.
RP Gillett, NP (reprint author), Univ Victoria, Environm & Climate Change Canada, Canadian Ctr Climate Modelling & Anal, Victoria, BC V8W 2Y2, Canada.
EM nathan.gillett@canada.ca
RI Funke, Bernd/C-2162-2008; Matthes, Katja/F-7361-2014; Shiogama,
Hideo/B-9598-2012; Knutti, Reto/B-8763-2008; Santer,
Benjamin/F-9781-2011
OI Funke, Bernd/0000-0003-0462-4702; Matthes, Katja/0000-0003-1801-3072;
Shiogama, Hideo/0000-0001-5476-2148; Knutti, Reto/0000-0001-8303-6700;
NR 76
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U1 11
U2 11
PU COPERNICUS GESELLSCHAFT MBH
PI GOTTINGEN
PA BAHNHOFSALLEE 1E, GOTTINGEN, 37081, GERMANY
SN 1991-959X
EI 1991-9603
J9 GEOSCI MODEL DEV
JI Geosci. Model Dev.
PD OCT 18
PY 2016
VL 9
IS 10
BP 3685
EP 3697
DI 10.5194/gmd-9-3685-2016
PG 13
WC Geosciences, Multidisciplinary
SC Geology
GA EA4LV
UT WOS:000386585100001
ER
PT J
AU Basu, A
Schilling, K
Brown, ST
Johnson, TM
Christensen, JN
Hartmann, M
Reimus, PW
Heikoop, JM
Woldegabriel, G
DePaolo, DJ
AF Basu, Anirban
Schilling, Kathrin
Brown, Shaun T.
Johnson, Thomas M.
Christensen, John N.
Hartmann, Matt
Reimus, Paul W.
Heikoop, Jeffrey M.
Woldegabriel, Giday
DePaolo, Donald J.
TI Se Isotopes as Groundwater Redox Indicators: Detecting Natural
Attenuation of Se at an in Situ Recovery U Mine
SO ENVIRONMENTAL SCIENCE & TECHNOLOGY
LA English
DT Article
ID URANIUM DEPOSITS; WATER-QUALITY; SELENIUM; REDUCTION; FRACTIONATION;
MAGNETITE; ACCUMULATION; MACKINAWITE; MOBILITY; SORPTION
AB One of the major ecological concerns associated with the in situ recovery (ISR) of uranium (U) is the environmental release of soluble, toxic selenium (Se) oxyanions generated by mining. Post-mining natural attenuation by the residual reductants in the ore body and reduced down gradient sediments should mitigate the risk of Se contamination in groundwater. In this work, we investigate the Se concentrations and Se isotope systematics of groundwater and of U ore bearing sediments from an ISR site at Rosita, TX, USA. Our results show that selenate (Se(VI)) is the dominant Se species in Rosita groundwater, and while several up-gradient wells have elevated Se(VI), the majority of the ore zone and down-gradient wells have little or no Se oxyanions. In addition, the delta(SeVI)-Se-82 of Rosita groundwater is generally elevated relative to the U ore up to +6.14 parts per thousand, with the most enriched values observed in the ore-zone wells. Increasing delta Se-82 with decreasing Se(VI) conforms to a Rayleigh type distillation model with an epsilon of -2.25% +/- 0.61 parts per thousand, suggesting natural Se(VI) reduction occurring along the hydraulic gradient at the Rosita ISR site. Furthermore, our results show that Se isotopes are excellent sensors, for detecting and, monitoring post-mining natural attenuation of Se oxyanions at ISR sites.
C1 [Basu, Anirban; Brown, Shaun T.; DePaolo, Donald J.] Univ Calif Berkeley, Dept Earth & Planetary Sci, 307 McCone Hall, Berkeley, CA 94720 USA.
[Schilling, Kathrin] Univ Calif Berkeley, Dept Environm Sci Policy & Management, 130 Mulford Hall, Berkeley, CA 94720 USA.
[Brown, Shaun T.; Christensen, John N.; DePaolo, Donald J.] Lawrence Berkeley Natl Lab, 1 Cyclotron Rd, Berkeley, CA 94720 USA.
[Johnson, Thomas M.] Univ Illinois, Dept Geol, 605 East Springfield Ave, Champaign, IL 61820 USA.
[Hartmann, Matt] Uranium Resources Inc, 6950 South Potomac St,Suite 300, Centennial, CO 80112 USA.
[Reimus, Paul W.; Heikoop, Jeffrey M.; Woldegabriel, Giday] Los Alamos Natl Lab, Earth & Environm Sci Div, Los Alamos, NM 87545 USA.
[Basu, Anirban] Royal Holloway Univ London, Dept Earth Sci, Egham Hill, Egham TW20 0EX, Surrey, England.
RP Basu, A (reprint author), Univ Calif Berkeley, Dept Earth & Planetary Sci, 307 McCone Hall, Berkeley, CA 94720 USA.; Basu, A (reprint author), Royal Holloway Univ London, Dept Earth Sci, Egham Hill, Egham TW20 0EX, Surrey, England.
EM Anirban.Basu@rhul.ac.uk
RI Brown, Shaun/E-9398-2015;
OI Brown, Shaun/0000-0002-2159-6718; Heikoop, Jeffrey/0000-0001-7648-3385;
Basu, Anirban/0000-0002-4905-9156
FU UC Laboratory Fees Research Program; U.S. Department of Energy
[DE-AC02-05CH11231]
FX This research was funded by the UC Laboratory Fees Research Program. We
thank Uranium Resources, Inc. for providing site access and logistic
support during sample collection and drilling. The U.S. Department of
Energy provided salary support for D.J.D. and J.N.C. during the study
period under contract no. DE-AC02-05CH11231. We thank two anonymous
reviewers and Associate Editor Daniel Giammar for constructive comments
that improved the quality of this manuscript.
NR 51
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U1 20
U2 20
PU AMER CHEMICAL SOC
PI WASHINGTON
PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA
SN 0013-936X
EI 1520-5851
J9 ENVIRON SCI TECHNOL
JI Environ. Sci. Technol.
PD OCT 18
PY 2016
VL 50
IS 20
BP 10833
EP 10842
DI 10.1021/acs.est.6b01464
PG 10
WC Engineering, Environmental; Environmental Sciences
SC Engineering; Environmental Sciences & Ecology
GA DZ5MW
UT WOS:000385907200008
ER
PT J
AU Olsen, TA
Brandt, CC
Brooks, SC
AF Olsen, Todd A.
Brandt, Craig C.
Brooks, Scott C.
TI Periphyton Biofilms Influence Net Methylmercury Production in an
Industrially Contaminated System
SO ENVIRONMENTAL SCIENCE & TECHNOLOGY
LA English
DT Article
ID MERCURY METHYLATION; PHOTOSYNTHESIS; MACROPHYTES; SEDIMENTS; TRACER;
WATER; CYCLE; MAT
AB Mercury (Hg) methylation and methylmercury (MMHg) demethylation activity of periphyton biofilms from the industrially contaminated East Fork Poplar Creek, Tennessee (EFPC) were measured during 2014-2016 using stable Hg isotopic rate assays. Hg-201(II) and (MMHg)-Hg-202 were added to intact periphyton samples in ambient streamwater and the formation of (MMHg)-Hg-201 and loss of (MMHg)-Hg-202, were monitored over time and used to calculate first-order rate potentials for methylation arid demethylation. The influences of location, temperature/season, light exposure and biofilm structure on methylation and demethylation potentials were examined. Between-site differences in net methylation for samples collected from an upstream versus downstream location were driven by differences in the demethylation rate potential (k(d)). In contrast, the within-site temperature-dependent difference in net methylation was driven by changes in the methylation rate potential. (k(m)). Samples incubated in the dark had lower net methylation due to lower k(m) values than those incubated in the light. Disrupting the biofilm structure decreased k(m) and resulted in lower net methylation. Overall, the measured rates resulted in a net excess of MMHg generated which could account for 3.71-7.88 mg d(-1) MMHg flux in EFPC and suggests intact, actively photosynthesizing periphyton biofilms harbor zones of MMHg production.
C1 [Olsen, Todd A.; Brooks, Scott C.] Oak Ridge Natl Lab, Div Environm Sci, POB 2008,MS 6038, Oak Ridge, TN 37831 USA.
[Brandt, Craig C.] Oak Ridge Natl Lab, Biosci Div, POB 2008,MS 6038, Oak Ridge, TN 37831 USA.
RP Brooks, SC (reprint author), Oak Ridge Natl Lab, Div Environm Sci, POB 2008,MS 6038, Oak Ridge, TN 37831 USA.
EM brookssc@ornl.gov
FU U.S. Department of Energy, Office of Science, Biological and
Environmental Research, Subsurface Biogeochemical Research Program; U.S.
Department of Energy [DE-AC05-000R22725]; DOE Public Access Plan
FX This work was funded by the U.S. Department of Energy, Office of
Science, Biological and Environmental Research, Subsurface
Biogeochemical Research Program and is a product of the Science Focus
Area (SFA) at ORNL. The isotopes used in this research were supplied by
the United States Department of Energy Office of Science by the Isotope
Program in the Office of Nuclear Physics. We thank Xiangping Yin for
help with sample analysis and Kenneth Lowe for help with constructing
the periphyton growth platforms, sample collection, and sample analysis.
A. Riscassi and four anonymous reviewers provided comments on earlier
versions of this manuscript that greatly improved the final version.
This manuscript has been authored by UT-Battelle, LLC under Contract No.
DE-AC05-000R22725 with the U.S. Department of Energy. The United States
Government retains and the publisher, by accepting the article for
publication, acknowledges that the United States Government retains a
nonexclusive, paid up, irrevocable, worldwide license to publish or
reproduce the published form of this manuscript, or allow others to do
so, for United States Government purposes. The Department of Energy will
provide public access to these results of federally sponsored research
in accordance with the DOE Public Access Plan
(http://energy.gov/downloads/doe-public-access-plan).
NR 36
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U1 19
U2 19
PU AMER CHEMICAL SOC
PI WASHINGTON
PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA
SN 0013-936X
EI 1520-5851
J9 ENVIRON SCI TECHNOL
JI Environ. Sci. Technol.
PD OCT 18
PY 2016
VL 50
IS 20
BP 10843
EP 10850
DI 10.1021/acs.est.6b01538
PG 8
WC Engineering, Environmental; Environmental Sciences
SC Engineering; Environmental Sciences & Ecology
GA DZ5MW
UT WOS:000385907200009
PM 27617484
ER
PT J
AU Sheng, AX
Liu, F
Shi, L
Liu, J
AF Sheng, Anxu
Liu, Feng
Shi, Liang
Liu, Juan
TI Aggregation Kinetics of Hematite Particles in the Presence of Outer
Membrane Cytochrome OmcA of Shewanella oneidenesis MR-1
SO ENVIRONMENTAL SCIENCE & TECHNOLOGY
LA English
DT Article
ID CRITICAL COAGULATION CONCENTRATION; ELECTRON-TRANSFER; NANOPARTICLES;
PROTEINS; NANOMATERIALS; STABILITY; SYSTEMS; SURFACE; SIZE; MTRC
AB The aggregation behavior of 9, 36, and 112 nm hematite particles was studied in the presence of OmcA, a bacterial extracellular protein, in aqueous dispersions at pH 5.7 through time-resolved dynamic light scattering, electrophoretic mobility, and circular dichroism spectra, respectively. At low salt concentration, the attachment efficiencies of hematite particles in all sizes first increased, then decreased, and finally remained stable with the increase of OmcA concentration, indicating the dominant interparticle interaction changed along with the increase in the protein-to-particle ratio. Nevertheless, at high salt concentration, the attachment efficiencies of all hematite samples gradually decreased with increasing OmcA concentration, which can be attributed to increasing steric force. Additionally, the aggregation behavior of OmcA-hematite conjugates was more correlated to total particle-surface area than primary particle size. It was further established that OmcA could stabilize hematite nanoparticles more efficiently than bovine serum albumin (BSA), a model plasma protein, due to the higher affinity of OmcA to hematite surface. This study highlighted the effects of particle properties, solution conditions, and protein properties on the complicated aggregation behavior of protein-nanoparticle conjugates in aqueous environments.
C1 [Sheng, Anxu; Liu, Feng; Liu, Juan] Peking Univ, Coll Environm Sci & Engn, Key Lab Water & Sediment Sci, Minist Educ, Beijing 100871, Peoples R China.
[Shi, Liang] China Univ Geosci, Sch Environm Studies, Dept Biol Sci & Technol, Wuhan 430074, Hubei, Peoples R China.
[Shi, Liang] Pacific Northwest Natl Lab, Richland, WA 99352 USA.
RP Liu, J (reprint author), Peking Univ, Coll Environm Sci & Engn, Key Lab Water & Sediment Sci, Minist Educ, Beijing 100871, Peoples R China.
EM juan.liu@pku.edu.cn
RI Liu, Juan/G-6035-2016
FU National Natural Science Foundation of China [41472306]; National Basic
Research Program of China (973 Program) [2014CB846001]
FX This work was financially supported by National Natural Science
Foundation of China (41472306) and the National Basic Research Program
of China (973 Program, 2014CB846001). We also thank Xinxin Wang for help
with the measurements of CD spectra.
NR 46
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U1 20
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PU AMER CHEMICAL SOC
PI WASHINGTON
PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA
SN 0013-936X
EI 1520-5851
J9 ENVIRON SCI TECHNOL
JI Environ. Sci. Technol.
PD OCT 18
PY 2016
VL 50
IS 20
BP 11016
EP 11024
DI 10.1021/acs.est.6b02963
PG 9
WC Engineering, Environmental; Environmental Sciences
SC Engineering; Environmental Sciences & Ecology
GA DZ5MW
UT WOS:000385907200028
ER
PT J
AU Zeng, XF
Borole, AP
Paylostathis, SG
AF Zeng, Xiaofei
Borole, Abhijeet P.
Paylostathis, Spyros G.
TI Inhibitory Effect of Furanic and Phenolic Compounds on Exoelectrogenesis
in a Microbial Electrolysis Cell Bioanode
SO ENVIRONMENTAL SCIENCE & TECHNOLOGY
LA English
DT Article
ID ETHANOLOGENIC ESCHERICHIA-COLI; ANODE-RESPIRING BACTERIA;
HYDROGEN-PRODUCTION; MIXED CULTURES; FERMENTATION; MECHANISMS;
GENERATION; TRANSPORT; BIOMASS; GROWTH
AB The objective of this study was to systematically investigate the inhibitory effect of furfural (FF), 5-hydroxymethylfurfural (HMF), syringic acid (SA), vanillic acid (VA), and 4-hydroxybenzoic acid (HBA); which are problematic lignocellulose-derived byproducts, on exoelectrogenesis in the bioanode of a microbial electrolysis cell. The five compound mixture at an initial total concentration range from 0.8 to 8.0 g/L resulted in an up to 91% current decrease as a result of exoelectrogenesis inhibition; fermentative, nonexoelectrogenic biotransformation pathways of the five compounds were not affected. Furthermore, the parent compounds at a high concentration, as opposed to their biotransformation products, were responsible for the observed inhibition. All five parent compounds contributed to the observed inhibition of the mixture. The IC50 (i.e., concentration resulting in 50% current decrease) of individually tested parent compounds was 2.7 g/L for FF, 3.0 g/L for HMF, 1.9 g/L for SA, 2.1 g/L for VA and 2.0 g/L for HBA. However,the parent compounds, when tested below their respective noninhibitory concentration, jointly resulted in significant inhibition as a mixture. Catechol and phenol, which were persistent biotransformation products, inhibited exoelectrogenesis only at high concentrations, but to a lesser extent than the parent compounds. Exoelectrogenesis recovery from inhibition by all compounds was observed at different rates, with the exception of catechol, which resulted in irreversible inhibition.
C1 [Zeng, Xiaofei; Paylostathis, Spyros G.] Georgia Inst Technol, Sch Civil & Environm Engn, Atlanta, GA 30332 USA.
[Borole, Abhijeet P.] Oak Ridge Natl Lab, Biosci Div, Oak Ridge, TN 37831 USA.
[Borole, Abhijeet P.] Univ Tennessee, Bredesen Ctr Interdisciplinary Res & Educ, Knoxville, TN 37996 USA.
RP Paylostathis, SG (reprint author), Georgia Inst Technol, Sch Civil & Environm Engn, Atlanta, GA 30332 USA.
EM spyros.pavlostathis@ce.gatech.edu
OI Borole, Abhijeet/0000-0001-8423-811X
FU U.S. Department of Energy, BioEnergy Technologies Office under the
Carbon, Hydrogen and Separations Efficiency (CHASE) in Bio-Oil
Conversion Pathways program [DE-FOA-0000812]; U.S. Department of Energy
[DEAC05-00OR22725]; DOE Public Access Plan
FX We acknowledge funding for this work from the U.S. Department of Energy,
BioEnergy Technologies Office under the Carbon, Hydrogen and Separations
Efficiency (CHASE) in Bio-Oil Conversion Pathways program,
DE-FOA-0000812. The manuscript has been coauthored by UT-Battelle, LLC,
under Contract DEAC05-00OR22725 with the U.S. Department of Energy. The
United States Government retains and the publisher, by accepting the
article for publication, acknowledges that the United States Government
retains a nonexclusive, paid up, irrevocable, worldwide license to
publish or reproduce the published form of this manuscript, or allow
others to do so, for United States Government purposes. The Department
of Energy will provide public access to these results of federally
sponsored research in accordance with the DOE Public Access Plan
(http://energy.gov/downloads/doe-public-access-plan).
NR 31
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U1 8
U2 8
PU AMER CHEMICAL SOC
PI WASHINGTON
PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA
SN 0013-936X
EI 1520-5851
J9 ENVIRON SCI TECHNOL
JI Environ. Sci. Technol.
PD OCT 18
PY 2016
VL 50
IS 20
BP 11357
EP 11365
DI 10.1021/acs.est.6b01505
PG 9
WC Engineering, Environmental; Environmental Sciences
SC Engineering; Environmental Sciences & Ecology
GA DZ5MW
UT WOS:000385907200066
PM 27611022
ER
PT J
AU Hellebrandt, S
Lee, SS
Knope, KE
Lussier, AJ
Stubbs, JE
Eng, PJ
Soderholm, L
Fenter, P
Schmidt, M
AF Hellebrandt, Stefan
Lee, Sang Soo
Knope, Karah E.
Lussier, Aaron J.
Stubbs, Joanne E.
Eng, Peter J.
Soderholm, L.
Fenter, Paul
Schmidt, Moritz
TI A Comparison of Adsorption, Reduction, and Polymerization of the
Plutonyl(VI) and Uranyl(VI) Ions from Solution onto the Muscovite Basal
Plane
SO LANGMUIR
LA English
DT Article
ID X-RAY REFLECTIVITY; PLUTONIUM OXIDE NANOPARTICLES; SURFACE-MEDIATED
REDUCTION; (001)-SOLUTION INTERFACE; 2ND-HARMONIC GENERATION;
SPECTROSCOPIC EVIDENCE; ELECTROLYTE-SOLUTIONS; REDOX SPECIATION;
HYDRATION FORCES; WATER-STRUCTURE
AB X-ray scattering techniques [in situ resonant anomalous X-ray reflectivity (RAXR) and specular crystal truncation rods (CTR)] were used to compare muscovite (001) surfaces in contact with solutions containing either 0.1 mM plutonyl(VI) or 1 mM uranyl(VI) at pH = 3.2 +/- 0.2, I(NaCl) = 0.1 M, as well as in situ grazing-incidence X-ray absorption near-edge structure (GI XANES) spectroscopy and ex situ alpha spectrometry. Details of the surface coverage are found to be very different. In the case of Pu, alpha spectrometry finds a surface coverage of 8.3 Pu/A(UC) (A(UC) = 46.72 angstrom(2), the unit cell area), far in excess of the 0.5 Pu/A(UC) expected for ionic adsorption of PuO22+. GI XANES results show that Pu is predominantly tetravalent on the surface, and the CTR/RAXR results show that the adsorbed Pu is broadly distributed. Taken together with previous findings, the results are consistent with adsorption of Pu in the form of Pu(IV)-oxo-nanoparticles. In contrast, uranyl shows only negligible, if any, adsorption according to all methods applied. These results are discussed and compared within the context of known Pu and U redox chemistry.
C1 [Hellebrandt, Stefan; Schmidt, Moritz] Helmholtz Zentrum Dresden Rossendorf, Inst Resource Ecol, D-01314 Dresden, Germany.
[Lee, Sang Soo; Knope, Karah E.; Soderholm, L.; Fenter, Paul] Argonne Natl Lab, Chem Sci & Engn Div, 9700 S Cass Ave, Argonne, IL 60439 USA.
[Lussier, Aaron J.] Univ Notre Dame, Dept Civil & Environm Engn & Earth Sci, Notre Dame, IN 46556 USA.
[Stubbs, Joanne E.; Eng, Peter J.] Univ Chicago, Ctr Adv Radiat Sources, Chicago, IL 60637 USA.
[Knope, Karah E.] Georgetown Univ, Dept Chem, Washington, DC 20057 USA.
RP Schmidt, M (reprint author), Helmholtz Zentrum Dresden Rossendorf, Inst Resource Ecol, D-01314 Dresden, Germany.; Soderholm, L (reprint author), Argonne Natl Lab, Chem Sci & Engn Div, 9700 S Cass Ave, Argonne, IL 60439 USA.
EM ls@anl.gov; moritz.schmidt@hzdr.de
RI Stubbs, Joanne/F-9710-2013; Schmidt, Moritz/C-2610-2011
OI Stubbs, Joanne/0000-0002-8509-2009; Schmidt, Moritz/0000-0002-8419-0811
FU Helmholtz Gemeinschaft Deutscher Forschungszentren [VH-NG-942]; U.S.
Department of Energy, Office of Science, Office of Basic Energy
Sciences, Chemical Sciences, Geosciences, and Biosciences Division
[DE-AC02-06CH11357]; Geoscience research program; Chemical Sciences
program; National Science Foundation-Earth Sciences [EAR-1128799];
Department of Energy-Geosciences [DE-FG02-94ER14466]
FX We thank Dr. S. Skanthakumar for his assistance in the preparation of XR
samples. This work was cofinanced (M.S. and S.H.) by the Helmholtz
Gemeinschaft Deutscher Forschungszentren by supporting the
Helmholtz-Nachwuchs-gruppe "Structures and Reactivity at the
Water/Mineral Interface" (VH-NG-942). Work conducted at Argonne National
Laboratory, operated by UChicago Argonne, LLC, was funded by the U.S.
Department of Energy, Office of Science, Office of Basic Energy
Sciences, Chemical Sciences, Geosciences, and Biosciences Division under
contract number DE-AC02-06CH11357, by the Geoscience (S.S.L. and P.F.)
and Chemical Sciences (K.E.K. and L.S.) research programs. The X-ray
data were collected at the GeoSoilEnviroCARS beamline 13-ID-C at the
Advanced Photon Source (APS), Argonne National Laboratory.
GeoSoilEnviro-CARS is supported by the National Science Foundation-Earth
Sciences (EAR-1128799) and Department of Energy-Geosciences
(DE-FG02-94ER14466) (J.E.S. and P.J.E.).
NR 83
TC 0
Z9 0
U1 9
U2 9
PU AMER CHEMICAL SOC
PI WASHINGTON
PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA
SN 0743-7463
J9 LANGMUIR
JI Langmuir
PD OCT 18
PY 2016
VL 32
IS 41
BP 10473
EP 10482
DI 10.1021/acs.langmuir.6b02513
PG 10
WC Chemistry, Multidisciplinary; Chemistry, Physical; Materials Science,
Multidisciplinary
SC Chemistry; Materials Science
GA DZ5ND
UT WOS:000385907900004
ER
PT J
AU Jung, H
Lee, B
Jun, YS
AF Jung, Haesung
Lee, Byeongdu
Jun, Young-Shin
TI Structural Match of Heterogeneously Nucleated Mn(OH)(2)(s) Nanoparticles
on Quartz under Various pH Conditions
SO LANGMUIR
LA English
DT Article
ID OXIDATION-REDUCTION EQUILIBRIA; TRANSITION-METAL OXIDES; INTERFACIAL
ENERGIES; MINERAL SURFACES; MANGANESE OXIDES; IONIC-STRENGTH; GROWTH;
BIRNESSITE; THERMODYNAMICS; MECHANISMS
AB The early nucleation stage of Mn (hydr)oxide on mineral surfaces is crucial to understand its occurrence and the cycling of nutrients in environmental systems. However, there are only limited studies on the heterogeneous nucleation of Mn(OH)(2)(s) as the initial stage of Mn (hydr)oxide precipitation. Here, we investigated the effect of pH on the initial nucleation of Mn(OH)(2)(s) on quartz. Under various pH conditions of 9.8, 9.9, and 10.1, we analyzed the structural matches between quartz and heterogeneously nucleated Mn(OH)(2)(s). The structural matches were calculated by measuring the lateral and vertical dimensions using grazing incidence small angle X-ray scattering and atomic force microscopy (AFM), respectively. We found that a poorer structural match occurred at a higher pH than at a lower pH. The faster nucleation under a higher pH condition accounted for the poorer structural match observed. By fitting the structural match using classical nucleation theory, we also calculated the interfacial energy between Mn(OH)(2)(s) and water: gamma(nf) = 71 +/- 7 mJ/m(2). The calculated m values and gamma(nf) provided the variance of interfacial energy between quartz and Mn(OH)(2)(s): gamma(sn) = 262-272 mJ/m(2). This study provides new qualitative and quantitative information on heterogeneous nucleation on an environmentally abundant mineral surface, quartz, and it offers important underpinnings for understanding the fate and transport of trace ions in environmental systems.
C1 [Jung, Haesung; Jun, Young-Shin] Washington Univ, Dept Energy Environm & Chem Engn, One Brookings Dr,Campus Box 1180, St Louis, MO 63130 USA.
[Lee, Byeongdu] Argonne Natl Lab, Xray Sci Div, 9700 S Cass Ave, Argonne, IL 60439 USA.
RP Jun, YS (reprint author), Washington Univ, Dept Energy Environm & Chem Engn, One Brookings Dr,Campus Box 1180, St Louis, MO 63130 USA.
EM ysjun@seas.wustl.edu
FU National Science Foundation's Environmental Chemical Sciences program
[CHE-1610728]; US Department of Energy, Office of Science, Office of
Basic Energy Sciences [DE-AC02-06CH11357]
FX The authors would like to acknowledge the support from the National
Science Foundation's Environmental Chemical Sciences program
(CHE-1610728). We also thank Washington University's Institute of
Materials Science and Engineering (IMSE) for the use of XPS, and
Professor James C. Ballard for carefully reviewing the manuscript. Use
of the Advanced Photon Source (APS) (Sector 12ID-B) at the Argonne
National Laboratory was supported by the US Department of Energy, Office
of Science, Office of Basic Energy Sciences, under Contract No.
DE-AC02-06CH11357.
NR 41
TC 1
Z9 1
U1 5
U2 5
PU AMER CHEMICAL SOC
PI WASHINGTON
PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA
SN 0743-7463
J9 LANGMUIR
JI Langmuir
PD OCT 18
PY 2016
VL 32
IS 41
BP 10735
EP 10743
DI 10.1021/acs.langmuir.6b02446
PG 9
WC Chemistry, Multidisciplinary; Chemistry, Physical; Materials Science,
Multidisciplinary
SC Chemistry; Materials Science
GA DZ5ND
UT WOS:000385907900036
ER
PT J
AU Kumar, P
Sendelbach, S
Beck, MA
Freeland, JW
Wang, Z
Wang, H
Yu, CC
Wu, RQ
Pappas, DP
McDermott, R
AF Kumar, P.
Sendelbach, S.
Beck, M. A.
Freeland, J. W.
Wang, Zhe
Wang, Hui
Yu, Clare C.
Wu, R. Q.
Pappas, D. P.
McDermott, R.
TI Origin and Reduction of 1/f Magnetic Flux Noise in Superconducting
Devices
SO PHYSICAL REVIEW APPLIED
LA English
DT Article
ID QUANTUM; SURFACES
AB Magnetic flux noise is a dominant source of dephasing and energy relaxation in superconducting qubits. The noise power spectral density varies with frequency as 1/f(alpha), with alpha <= 1, and spans 13 orders of magnitude. Recent work indicates that the noise is from unpaired magnetic defects on the surfaces of the superconducting devices. Here, we demonstrate that adsorbed molecular O-2 is the dominant contributor to magnetism in superconducting thin films. We show that this magnetism can be reduced by appropriate surface treatment or improvement in the sample vacuum environment. We observe a suppression of static spin susceptibility by more than an order of magnitude and a suppression of 1/f magnetic flux noise power spectral density of up to a factor of 5. These advances open the door to the realization of superconducting qubits with improved quantum coherence.
C1 [Kumar, P.; Sendelbach, S.; Beck, M. A.; McDermott, R.] Univ Wisconsin, Dept Phys, 1150 Univ Ave, Madison, WI 53706 USA.
[Freeland, J. W.] Argonne Natl Lab, Adv Photon Source, Argonne, IL 60439 USA.
[Wang, Zhe; Wang, Hui; Yu, Clare C.; Wu, R. Q.] Univ Calif Irvine, Dept Phys & Astron, Irvine, CA 92617 USA.
[Wang, Zhe; Wang, Hui] Fudan Univ, State Key Lab Surface Phys, Shanghai 200433, Peoples R China.
[Wang, Zhe; Wang, Hui] Fudan Univ, Key Lab Computat Phys Sci, Shanghai 200433, Peoples R China.
[Pappas, D. P.] NIST, Boulder, CO 80305 USA.
[Sendelbach, S.] Northrop Grumman Corp, Linthicum, MD 21203 USA.
RP McDermott, R (reprint author), Univ Wisconsin, Dept Phys, 1150 Univ Ave, Madison, WI 53706 USA.
EM rfmcdermott@wisc.edu
FU U.S. Government [W911NF-09-1-0375, W911NF-10-1-0494]; DOE-BES
[DE-FG02-05ER46237]; NERSC; CNSF [11474056]; U.S. Department of Energy,
Office of Science [DEAC02-06CH11357]; LPS; ARO; DARPA
FX We thank M. Aiello, A. Puglielli, and T. Klaus for technical assistance
and we acknowledge useful discussions with J. L. DuBois, L. Faoro, L. B.
Ioffe, V. Lordi, and J. M. Martinis. This work is supported in part by
the U.S. Government under Grants No. W911NF-09-1-0375 and No.
W911NF-10-1-0494 and by a gift from Google, Inc. DFT calculations at UCI
(H. W. and R. Q. W.) are supported by DOE-BES (Grant No.
DE-FG02-05ER46237) and NERSC. Work at Fudan (Z. W. and R. Q. W.) is
supported by the CNSF (Grant No. 11474056). Work at the Advanced Photon
Source, Argonne is supported by the U.S. Department of Energy, Office of
Science under Grant No. DEAC02-06CH11357. NIST acknowledges support from
the LPS, ARO, and DARPA.
NR 24
TC 2
Z9 2
U1 4
U2 4
PU AMER PHYSICAL SOC
PI COLLEGE PK
PA ONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA
SN 2331-7019
J9 PHYS REV APPL
JI Phys. Rev. Appl.
PD OCT 18
PY 2016
VL 6
IS 4
PG 5
WC Physics, Applied
SC Physics
GA EA1ZB
UT WOS:000386389700001
ER
PT J
AU Szilard, D
Kort-Kamp, WJM
Rosa, FSS
Pinheiro, FA
Farina, C
AF Szilard, D.
Kort-Kamp, W. J. M.
Rosa, F. S. S.
Pinheiro, F. A.
Farina, C.
TI Purcell effect at the percolation transition
SO PHYSICAL REVIEW B
LA English
DT Article
ID ENHANCED RAMAN-SCATTERING; SPONTANEOUS EMISSION; OPTICAL-PROPERTIES;
MICROSCOPY; LIGHT; POLARIZATION; MOLECULE
AB We investigate the spontaneous emission rate of a two-level quantum emitter next to a composite medium made of randomly distributed metallic inclusions embedded in a dielectric host matrix. In the near field, the Purcell factor can be enhanced by two orders of magnitude relative to the case of a homogeneous metallic medium and reaches its maximum precisely at the insulator-metal transition. By unveiling the role of the decay pathways in the emitter's lifetime, we demonstrate that, close to the percolation threshold, the radiation emission process is dictated by electromagnetic absorption in the heterogeneous medium. We show that our findings are robust against change in material properties and shape of inclusions and apply for different effective-medium theories as well as for a wide range of transition frequencies.
C1 [Szilard, D.; Rosa, F. S. S.; Pinheiro, F. A.; Farina, C.] Univ Fed Rio de Janeiro, Inst Fis, Caixa Postal 68528, BR-21941972 Rio De Janeiro, Rio De Janeiro, Brazil.
[Kort-Kamp, W. J. M.] Los Alamos Natl Lab, Div Theoret, MS B258, Los Alamos, NM 87545 USA.
[Kort-Kamp, W. J. M.] Los Alamos Natl Lab, Ctr Nonlinear Studies, MS B258, Los Alamos, NM 87545 USA.
RP Szilard, D (reprint author), Univ Fed Rio de Janeiro, Inst Fis, Caixa Postal 68528, BR-21941972 Rio De Janeiro, Rio De Janeiro, Brazil.
RI PINHEIRO, FELIPE/L-3872-2016
OI PINHEIRO, FELIPE/0000-0001-8712-0555
FU CAPES [BEX 1497/14-6]; CNPq [303286/2013-0]; FAPERJ; LANL LDRD project;
CNLS; Royal Society (U.K.) through a Newton Advanced Fellowship
[NA150208]
FX We thank E. C. Marino and M. Hippert for useful discussions. D.S.,
F.S.S.R., and C.F. acknowledge CAPES, CNPq, and FAPERJ for financing
this research. W.J.M.K.-K. thanks the LANL LDRD project and CNLS for
financial support. F.A.P. thanks the Optoelectronics Research Centre and
Centre for Photonic Metamaterials, University of Southampton, where part
of this work was done, for hospitality and CAPES for funding his visit.
F.A.P. acknowledges the financial support of the Royal Society (U.K.)
through a Newton Advanced Fellowship (Ref. No. NA150208), CAPES (Grant
No. BEX 1497/14-6), and CNPq (Grant No. 303286/2013-0).
NR 39
TC 0
Z9 0
U1 8
U2 8
PU AMER PHYSICAL SOC
PI COLLEGE PK
PA ONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA
SN 2469-9950
EI 2469-9969
J9 PHYS REV B
JI Phys. Rev. B
PD OCT 18
PY 2016
VL 94
IS 13
AR 134204
DI 10.1103/PhysRevB.94.134204
PG 8
WC Physics, Condensed Matter
SC Physics
GA DZ8AK
UT WOS:000386090300002
ER
PT J
AU Jiang, Y
Lin, ZW
Liao, JF
AF Jiang, Yin
Lin, Zi-Wei
Liao, Jinfeng
TI Rotating quark-gluon plasma in relativistic heavy-ion collisions
SO PHYSICAL REVIEW C
LA English
DT Article
ID ENERGY NUCLEAR COLLISIONS; QCD MATTER; VIOLATION
AB We study the rotational collective motion of the quark-gluon plasma in relativistic heavy-ion collisions using the widely adopted a multiphase transport (AMPT) model. The global angular momentum, the average vorticity carried by the quark-gluon plasma, and the locally defined vorticity fields are computed for Au + Au collisions, with detailed information of their time evolution, spatial distribution, as well as the dependence on beam energy and collision centrality.
C1 [Jiang, Yin; Liao, Jinfeng] Indiana Univ, Dept Phys, 2401 North Milo B Sampson Lane, Bloomington, IN 47408 USA.
[Jiang, Yin; Liao, Jinfeng] Indiana Univ, Ctr Explorat Energy & Matter, 2401 North Milo B Sampson Lane, Bloomington, IN 47408 USA.
[Lin, Zi-Wei] East Carolina Univ, Dept Phys, Greenville, NC 27858 USA.
[Liao, Jinfeng] RIKEN, BNL Res Ctr, Brookhaven Natl Lab, Bldg 510A, Upton, NY 11973 USA.
RP Jiang, Y (reprint author), Indiana Univ, Dept Phys, 2401 North Milo B Sampson Lane, Bloomington, IN 47408 USA.; Jiang, Y (reprint author), Indiana Univ, Ctr Explorat Energy & Matter, 2401 North Milo B Sampson Lane, Bloomington, IN 47408 USA.
FU U.S. Department of Energy, Office of Science, Office of Nuclear Physics,
within the framework of the Beam Energy Scan Theory (BEST) Topical
Collaboration; US National Science Foundation [PHY-1352368]; RIKEN BNL
Research Center
FX The authors thank H. Huang, X. G. Huang, D. Kharzeev, M. Lisa, A. Tang,
F. Wang, G. Wang, N. Xu, and Z. Xu for helpful discussions. This
material is based upon work supported by the U.S. Department of Energy,
Office of Science, Office of Nuclear Physics, within the framework of
the Beam Energy Scan Theory (BEST) Topical Collaboration. The research
of J.L. is also supported in part by the US National Science Foundation
(Grant No. PHY-1352368) and by the RIKEN BNL Research Center. J.L.
acknowledges the Simons Center for Geometry and Physics, Stony Brook
University, at which some of the research for this paper was performed.
NR 36
TC 4
Z9 4
U1 2
U2 2
PU AMER PHYSICAL SOC
PI COLLEGE PK
PA ONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA
SN 2469-9985
EI 2469-9993
J9 PHYS REV C
JI Phys. Rev. C
PD OCT 18
PY 2016
VL 94
IS 4
AR 044910
DI 10.1103/PhysRevC.94.044910
PG 9
WC Physics, Nuclear
SC Physics
GA DZ9CH
UT WOS:000386170300003
ER
PT J
AU Rehm, KE
Esbensen, H
Jiang, CL
Back, BB
Stefanini, AM
Montagnoli, G
AF Rehm, K. E.
Esbensen, H.
Jiang, C. L.
Back, B. B.
Stefanini, A. M.
Montagnoli, G.
TI Moments of fusion-barrier distributions
SO PHYSICAL REVIEW C
LA English
DT Article
ID HEAVY-ION FUSION; AVERAGE ANGULAR MOMENTA; SUBBARRIER FUSION;
CROSS-SECTIONS; COULOMB BARRIER; NI-58; NI-64
AB A study of fusion-barrier distributions through an analysis of their moments is presented. The moments can be obtained from least-squares fits of the energy-weighted fusion cross sections without the need of calculating second derivatives. The zeroth and first moments determine the fusion radius R and the Coulomb barrier V-C. These two quantities are the same as the parameters R and V-C that are used in the well-known expression, E sigma = pi R-2(E - V-C), for the fusion cross section at high energies. The second and third moments, M-2 and M-3, determine the width and skewness of the barrier distribution, respectively. From these global parameters new correlations for the study of heavy-ion-induced fusion reactions can be obtained. Systems exhibiting a large coupling to transfer reactions show a small fusion radius as well as a large second moment. A negative third moment is correlated with a prolate deformation of the target nucleus.
C1 [Rehm, K. E.; Esbensen, H.; Jiang, C. L.; Back, B. B.] Argonne Natl Lab, Div Phys, Argonne, IL 60439 USA.
[Stefanini, A. M.] INFN, Lab Nazl Legnaro, I-35020 Legnaro, Padova, Italy.
[Montagnoli, G.] Univ Padua, Dipartimento Fis & Astron, I-35131 Padua, Italy.
[Montagnoli, G.] INFN, Sez Padova, I-35131 Padua, Italy.
RP Rehm, KE (reprint author), Argonne Natl Lab, Div Phys, Argonne, IL 60439 USA.
FU US Department of Energy, Office of Science, Office of Nuclear Physics
[DE-AC02-06CH11357]; European Union Seventh Framework Programme FP7
[262010-ENSAR]
FX This work was supported by the US Department of Energy, Office of
Science, Office of Nuclear Physics, under Contract No. DE-AC02-06CH11357
and the European Union Seventh Framework Programme FP7/2007-2013 under
Grant No. 262010-ENSAR.
NR 47
TC 0
Z9 0
U1 3
U2 3
PU AMER PHYSICAL SOC
PI COLLEGE PK
PA ONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA
SN 2469-9985
EI 2469-9993
J9 PHYS REV C
JI Phys. Rev. C
PD OCT 18
PY 2016
VL 94
IS 4
AR 044612
DI 10.1103/PhysRevC.94.044612
PG 8
WC Physics, Nuclear
SC Physics
GA DZ9CH
UT WOS:000386170300002
ER
PT J
AU Huang, PS
Long, AJ
Wang, LT
AF Huang, Peisi
Long, Andrew J.
Wang, Lian-Tao
TI Probing the electroweak phase transition with Higgs factories and
gravitational waves
SO PHYSICAL REVIEW D
LA English
DT Article
ID BARYOGENESIS; RADIATION; BOSON
AB After the discovery of the Higgs boson, understanding the nature of electroweak symmetry breaking and the associated electroweak phase transition has become the most pressing question in particle physics. Answering this question is a priority for experimental studies. Data from the LHC and future lepton collider-based Higgs factories may uncover new physics coupled to the Higgs boson, which can induce the electroweak phase transition to become first order. Such a phase transition generates a stochastic background of gravitational waves, which could potentially be detected by a space-based gravitational wave interferometer. In this paper, we survey a few classes of models in which the electroweak phase transition is strongly first order. We identify the observables that would provide evidence of these models at the LHC and next-generation lepton colliders, and we assess whether the corresponding gravitational wave signal could be detected by eLISA. We find that most of the models with first-order electroweak phase transition can be covered by the precise measurements of Higgs couplings at the proposed Higgs factories. We also map out the model space that can be probed with gravitational wave detection by eLISA.
C1 [Huang, Peisi; Long, Andrew J.; Wang, Lian-Tao] Univ Chicago, Enrico Fermi Inst, Chicago, IL 60637 USA.
[Huang, Peisi] Argonne Natl Lab, High Energy Phys Div, Argonne, IL 60439 USA.
[Wang, Lian-Tao] Univ Chicago, Kavli Inst Cosmol Phys, Chicago, IL 60637 USA.
RP Huang, PS (reprint author), Univ Chicago, Enrico Fermi Inst, Chicago, IL 60637 USA.; Huang, PS (reprint author), Argonne Natl Lab, High Energy Phys Div, Argonne, IL 60439 USA.
EM peisi@uchicago.edu; andrewjlong@kicp.uchicago.edu; liantaow@uchicago.edu
OI Huang, Peisi/0000-0003-3360-2641
FU U.S. Department of Energy [DE-AC02-06CH11357, DE-FG02-04ER41286]; Kavli
Institute for Cosmological Physics [NSF PHY-1125897]; Kavli Foundation;
Department of Energy (DOE) [DE-SC0013642]
FX We are grateful to Michael Fedderke for various discussions of the heavy
fermion model. We thank Jing Shu and Carlos Wagner for interesting
discussions. Work at Argonne National Laboratory (ANL) is supported in
part by the U.S. Department of Energy under Contract No.
DE-AC02-06CH11357. P. H. is partially supported by U.S. Department of
Energy Grant No. DE-FG02-04ER41286. A. J. L. is supported at the
University of Chicago by the Kavli Institute for Cosmological Physics
through Grant No. NSF PHY-1125897 and an endowment from the Kavli
Foundation and its founder Fred Kavli. L.-T. W. is supported by
Department of Energy (DOE) Grant No. DE-SC0013642.
NR 67
TC 0
Z9 0
U1 1
U2 1
PU AMER PHYSICAL SOC
PI COLLEGE PK
PA ONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA
SN 2470-0010
EI 2470-0029
J9 PHYS REV D
JI Phys. Rev. D
PD OCT 18
PY 2016
VL 94
IS 7
AR 075008
DI 10.1103/PhysRevD.94.075008
PG 17
WC Astronomy & Astrophysics; Physics, Particles & Fields
SC Astronomy & Astrophysics; Physics
GA DZ9CX
UT WOS:000386172100002
ER
PT J
AU Deng, L
Ibrahim, YM
Garimella, SVB
Webb, IK
Hamid, AM
Norheim, RV
Prost, SA
Sandoval, JA
Baker, ES
Smith, RD
AF Deng, Liulin
Ibrahim, Yehia M.
Garimella, Sandilya V. B.
Webb, Ian K.
Hamid, Ahmed M.
Norheim, Randolph V.
Prost, Spencer A.
Sandoval, Jeremy A.
Baker, Erin S.
Smith, Richard D.
TI Greatly Increasing Trapped Ion Populations for Mobility Separations
Using Traveling Waves in Structures for Lossless Ion Manipulations
SO ANALYTICAL CHEMISTRY
LA English
DT Article
ID FLIGHT MASS-SPECTROMETRY; ELECTROSPRAY-IONIZATION; FUNNEL TRAP;
RESOLUTION; PEPTIDE; BIOMOLECULES; INTERFACE; MIXTURES; MS
AB The initial use of traveling waves (TW) for ion mobility (TW) separations using structures for lossless ion manipulations (SLIM) employed an ion funnel trap (IFT) to accumulate ions from a continuous electrospray ionization source and was limited to injected ion populations of 406 charges due to the onset of space charge effects in the trapping region. Additional limitations arise due to the loss of resolution for the injection of ions over longer periods, such as in extended pulses. In this work a new SLIM "flat funnel" (FF) module has been developed and demonstrated to enable the accumulation of much larger ion populations and their injection for IM separations. Ion current measurements indicate a capacity: of similar to 3.2 X 10(8) charges for the extended trapping volume, over an order of magnitude greater than that of the IFT. The orthogonal ion injection into a funnel shaped separation region can greatly reduce space charge effects during the initial IM separation stage, and the gradually reduced width of the path allows the ion packet to be increasingly compresed in the lateral dimension as the, separation progresses, allowing efficient transmission through conductance limits or compatibility with subsequent ion manipulations. This work examined the TW, rf, and dc confining field SLIM parameters, involved in ion accumulation, injection, transmission, and IM separation in the FF module using both direct ion: current and MS measurements. Wide m/z range ion transmission is demonstrated, along with significant increases in the signal-to-noise ratios (S/N) due to the larger ion populations injected. Additionally, we observed a reduction in the chemical background, which was attributed to more efficient desolvatiori of solvent related clusters over the extended ion accumulation periods. The TW SLIM FF IM module is anticipated to be especially effective as a front end for long path SLIM IM separation modules.
C1 [Smith, Richard D.] Pacific Northwest Natl Lab, Div Biol Sci, Richland, WA 99352 USA.
Pacific Northwest Natl Lab, Environm Mol Sci Lab, Richland, WA 99352 USA.
RP Smith, RD (reprint author), Pacific Northwest Natl Lab, Div Biol Sci, Richland, WA 99352 USA.
EM rds@pnnl.gov
RI Smith, Richard/J-3664-2012;
OI Smith, Richard/0000-0002-2381-2349; Garimella, Sandilya Venkata
Bhaskara/0000-0001-6649-9842
FU National Institute of General Medical Sciences [P41 GM103493];
Laboratory Directed Research and Development Program at Pacific
Northwest National Laboratory; U.S. Department of Energy Office of
Biological and Environmental Research Genome Sciences Program under
Pan-omics Program; DOE [DE-AC05-76RL0 1830]
FX Portions of this research were supported by grants from the National
Institute of General Medical Sciences (Grant P41 GM103493), the
Laboratory Directed Research and Development Program at Pacific
Northwest National Laboratory, and the U.S. Department of Energy Office
of Biological and Environmental Research Genome Sciences Program under
the Pan-omics Program. This work was performed in the W. R. Wiley
Environmental Molecular Sciences Laboratory (EMSL), a DOE national
scientific user facility at the Pacific Northwest National Laboratory
(PNNL). PNNL is operated by Battelle for the DOE under Contract
DE-AC05-76RL0 1830.
NR 41
TC 2
Z9 2
U1 7
U2 7
PU AMER CHEMICAL SOC
PI WASHINGTON
PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA
SN 0003-2700
EI 1520-6882
J9 ANAL CHEM
JI Anal. Chem.
PD OCT 18
PY 2016
VL 88
IS 20
BP 10143
EP 10150
DI 10.1021/acs.analchem.6b02678
PG 8
WC Chemistry, Analytical
SC Chemistry
GA DZ5MY
UT WOS:000385907400038
ER
PT J
AU Templeton, DW
Sluiter, JB
Sluiter, A
Payne, C
Crocker, DP
Tao, L
Wolfrum, E
AF Templeton, David W.
Sluiter, Justin B.
Sluiter, Amie
Payne, Courtney
Crocker, David P.
Tao, Ling
Wolfrum, Ed
TI Long-term variability in sugarcane bagasse feedstock compositional
methods: sources and magnitude of analytical variability
SO BIOTECHNOLOGY FOR BIOFUELS
LA English
DT Article
DE Compositional analysis; Sugarcane bagasse; Variability; Biofuels; NIST
RM 8491; MESP
ID CELLULOSIC ETHANOL-PRODUCTION; CORN STOVER; LIGNOCELLULOSIC BIOMASS;
FERMENTATION; PRETREATMENT; HYDROLYSIS; BIOETHANOL; BIOFUELS
AB Background: In an effort to find economical, carbon-neutral transportation fuels, biomass feedstock compositional analysis methods are used to monitor, compare, and improve biofuel conversion processes. These methods are empirical, and the analytical variability seen in the feedstock compositional data propagates into variability in the conversion yields, component balances, mass balances, and ultimately the minimum ethanol selling price (MESP). We report the average composition and standard deviations of 119 individually extracted National Institute of Standards and Technology (NIST) bagasse [Reference Material (RM) 8491] run by seven analysts over 7 years. Two additional datasets, using bulk-extracted bagasse (containing 58 and 291 replicates each), were examined to separate out the effects of batch, analyst, sugar recovery standard calculation method, and extractions from the total analytical variability seen in the individually extracted dataset. We believe this is the world's largest NIST bagasse compositional analysis dataset and it provides unique insight into the long-term analytical variability. Understanding the long-term variability of the feedstock analysis will help determine the minimum difference that can be detected in yield, mass balance, and efficiency calculations.
Results: The long-term data show consistent bagasse component values through time and by different analysts. This suggests that the standard compositional analysis methods were performed consistently and that the bagasse RM itself remained unchanged during this time period. The long-term variability seen here is generally higher than short-term variabilities. It is worth noting that the effect of short-term or long-term feedstock compositional variability on MESP is small, about $0.03 per gallon.
Conclusions: The long-term analysis variabilities reported here are plausible minimum values for these methods, though not necessarily average or expected variabilities. We must emphasize the importance of training and good analytical procedures needed to generate this data. When combined with a robust QA/QC oversight protocol, these empirical methods can be relied upon to generate high-quality data over a long period of time.
C1 [Templeton, David W.; Sluiter, Justin B.; Sluiter, Amie; Payne, Courtney; Crocker, David P.; Tao, Ling; Wolfrum, Ed] Natl Renewable Energy Lab, Natl Bioenergy Ctr, 15013 Denver West Pkwy, Golden, CO 80401 USA.
RP Templeton, DW; Sluiter, JB (reprint author), Natl Renewable Energy Lab, Natl Bioenergy Ctr, 15013 Denver West Pkwy, Golden, CO 80401 USA.
EM David.Templeton@nrel.gov; Justin.Sluiter@nrel.gov
OI Wolfrum, Edward/0000-0002-7361-8931
FU US Department of Energy Bioenergy Technologies Office
FX This work was supported by the US Department of Energy Bioenergy
Technologies Office.
NR 30
TC 0
Z9 0
U1 7
U2 7
PU BIOMED CENTRAL LTD
PI LONDON
PA 236 GRAYS INN RD, FLOOR 6, LONDON WC1X 8HL, ENGLAND
SN 1754-6834
J9 BIOTECHNOL BIOFUELS
JI Biotechnol. Biofuels
PD OCT 18
PY 2016
VL 9
AR 223
DI 10.1186/s13068-016-0621-z
PG 12
WC Biotechnology & Applied Microbiology; Energy & Fuels
SC Biotechnology & Applied Microbiology; Energy & Fuels
GA DZ1EG
UT WOS:000385581100008
PM 27777625
ER
PT J
AU Intravaia, F
Behunin, RO
Henkel, C
Busch, K
Dalvit, DAR
AF Intravaia, F.
Behunin, R. O.
Henkel, C.
Busch, K.
Dalvit, D. A. R.
TI Non-Markovianity in atom-surface dispersion forces
SO PHYSICAL REVIEW A
LA English
DT Article
ID QUANTUM-STATISTICAL EQUILIBRIUM; DIMENSIONAL RADIATION-FIELD;
WIGNER-WEISSKOPF ATOM; IRREVERSIBLE-PROCESSES; SPONTANEOUS EMISSION;
REGRESSION THEOREM; RECIPROCAL RELATIONS; HEAT-TRANSFER; RELAXATION;
FLUCTUATIONS
AB We discuss the failure of the Markov approximation in the description of atom-surface fluctuation-induced interactions, both in equilibrium (Casimir-Polder forces) and out of equilibrium (quantum friction). Using general theoretical arguments, we show that the Markov approximation can lead to erroneous predictions of such phenomena with regard to both strength and functional dependencies on system parameters. In particular, we show that the long-time power-law tails of two-time dipole correlations and their corresponding low-frequency behavior, neglected in the Markovian limit, affect the prediction of the force. Our findings highlight the importance of non-Markovian effects in dispersion interactions.
C1 [Intravaia, F.; Busch, K.] Max Born Inst, D-12489 Berlin, Germany.
[Behunin, R. O.] Yale Univ, Dept Appl Phys, New Haven, CT 06511 USA.
[Henkel, C.] Univ Potsdam, Inst Phys & Astron, Karl Liebknecht Str 24-25, D-14476 Potsdam, Germany.
[Busch, K.] Humboldt Univ, Inst Phys, AG Theoret Opt & Photon, D-12489 Berlin, Germany.
[Dalvit, D. A. R.] Los Alamos Natl Lab, Div Theoret, MS B213, Los Alamos, NM 87545 USA.
RP Intravaia, F (reprint author), Max Born Inst, D-12489 Berlin, Germany.
FU LANL LDRD program; Deutsche Forschungsgemeinschaft (DFG) within the
Collaborative Research Center (CRC) Hybrid Inorganic/Organic Systems for
Opto-Electronics (HIOS) [B10, 951]; European Union
[PCIG14-GA-2013-631571]; DFG through the DIP program [SCHM 1049/7-1];
NSF MRSEC [DMR-1119826]; Packard Fellowship for Science and Engineering;
Yale University
FX We thank G. Barton, S. Buhmann, M. Donaire, B. Farias, J. Klatt, K.
Milton, D. Reiche, S. Scheel, and W.-K. Tse for useful discussions. We
acknowledge support by the LANL LDRD program, and by the Deutsche
Forschungsgemeinschaft (DFG) through Project No. B10 within the
Collaborative Research Center (CRC) 951 Hybrid Inorganic/Organic Systems
for Opto-Electronics (HIOS). F.I. further acknowledges financial support
from the European Union Marie Curie People program through the Career
Integration Grant No. PCIG14-GA-2013-631571. C.H. and F.I. acknowledge
support from the DFG through the DIP program (Grant No. SCHM 1049/7-1).
R.B. further acknowledges financial support provided by NSF MRSEC
DMR-1119826, the Packard Fellowship for Science and Engineering as well
as Yale University startup funding.
NR 84
TC 1
Z9 1
U1 6
U2 6
PU AMER PHYSICAL SOC
PI COLLEGE PK
PA ONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA
SN 2469-9926
EI 2469-9934
J9 PHYS REV A
JI Phys. Rev. A
PD OCT 18
PY 2016
VL 94
IS 4
AR 042114
DI 10.1103/PhysRevA.94.042114
PG 16
WC Optics; Physics, Atomic, Molecular & Chemical
SC Optics; Physics
GA DZ6OR
UT WOS:000385982300001
ER
PT J
AU Zhang, XM
Tajima, T
Farinella, D
Shin, YM
Mourou, G
Wheeler, J
Taborek, P
Chen, PS
Dollar, F
Shen, BF
AF Zhang, Xiaomei
Tajima, Toshiki
Farinella, Deano
Shin, Youngmin
Mourou, Gerard
Wheeler, Jonathan
Taborek, Peter
Chen, Pisin
Dollar, Franklin
Shen, Baifei
TI Particle-in-cell simulation of x-ray wakefield acceleration and betatron
radiation in nanotubes
SO PHYSICAL REVIEW ACCELERATORS AND BEAMS
LA English
DT Article
ID ELECTRON-BEAM; PLASMA; PHYSICS; CARBON; WAKE
AB Though wakefield acceleration in crystal channels has been previously proposed, x-ray wakefield acceleration has only recently become a realistic possibility since the invention of the single-cycled optical laser compression technique. We investigate the acceleration due to a wakefield induced by a coherent, ultrashort x-ray pulse guided by a nanoscale channel inside a solid material. By two-dimensional particle-in-cell computer simulations, we show that an acceleration gradient of TeV/cm is attainable. This is about 3 orders of magnitude stronger than that of the conventional plasma-based wakefield accelerations, which implies the possibility of an extremely compact scheme to attain ultrahigh energies. In addition to particle acceleration, this scheme can also induce the emission of high energy photons at similar to O(10-100) MeV. Our simulations confirm such high energy photon emissions, which is in contrast with that induced by the optical laser driven wakefield scheme. In addition to this, the significantly improved emittance of the energetic electrons has been discussed.
C1 [Zhang, Xiaomei; Shen, Baifei] Chinese Acad Sci, Shanghai Inst Opt & Fine Mech, Shanghai 201800, Peoples R China.
[Zhang, Xiaomei; Tajima, Toshiki; Farinella, Deano; Taborek, Peter; Dollar, Franklin] UC, Dept Phys & Astron, Irvine, CA 92697 USA.
[Shin, Youngmin] Northern Illinois Univ, De Kalb, IL 60115 USA.
[Shin, Youngmin] Fermilab Natl Accelerator Lab, De Kalb, IL 60115 USA.
[Mourou, Gerard; Wheeler, Jonathan] Ecole Polytech, DER IZEST, F-91128 Palaiseau, France.
[Chen, Pisin] Natl Taiwan Univ, Dept Phys, Taipei 10617, Taiwan.
[Chen, Pisin] Natl Taiwan Univ, Leung Ctr Cosmol & Particle Astrophys, Taipei 10617, Taiwan.
RP Zhang, XM (reprint author), Chinese Acad Sci, Shanghai Inst Opt & Fine Mech, Shanghai 201800, Peoples R China.; Zhang, XM (reprint author), UC, Dept Phys & Astron, Irvine, CA 92697 USA.
FU Norman Rostorker Fund; National Natural Science Foundation of China
[11374319, 11125526, 11335013, 11674339, 11127901]; Ministry of Science
and Technology of the People's Republic of China [2016YFA0401102];
Strategic Priority Research Program of the Chinese Academy of Sciences
[XDB16]; China Scholarship Council
FX The work has been supported by the Norman Rostorker Fund, and was
further supported by the National Natural Science Foundation of China
(Grants No. 11374319, No. 11125526, No. 11335013, No. 11674339 and No.
11127901), the Ministry of Science and Technology of the People's
Republic of China (Grant No. 2016YFA0401102), the Strategic Priority
Research Program of the Chinese Academy of Sciences (Grant No. XDB16),
and the China Scholarship Council. We thank the dedicated effort of
Extreme Light Infrastructure-Nuclear Physics in realization of the thin
film compression [49]. Toshiki Tajima thanks the Einstein Professorship
of the Chinese Academy of Science and Professor Ruxin Li for his
kindness to have hosted Toshiki Tajima as Einstein Professor, from which
this work started and which in part supported this work, including that
of Xiaomei Zhang.
NR 47
TC 2
Z9 2
U1 17
U2 17
PU AMER PHYSICAL SOC
PI COLLEGE PK
PA ONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA
SN 2469-9888
J9 PHYS REV ACCEL BEAMS
JI Phys. Rev. Accel. Beams
PD OCT 18
PY 2016
VL 19
IS 10
AR 101004
DI 10.1103/PhysRevAccelBeams.19.101004
PG 10
WC Physics, Nuclear; Physics, Particles & Fields
SC Physics
GA DZ6MY
UT WOS:000385977800001
ER
PT J
AU Kang, J
Wells, SA
Wood, JD
Lee, JH
Liu, XL
Ryder, CR
Zhu, J
Guest, JR
Husko, CA
Hersam, MC
AF Kang, Joohoon
Wells, Spencer A.
Wood, Joshua D.
Lee, Jae-Hyeok
Liu, Xiaolong
Ryder, Christopher R.
Zhu, Jian
Guest, Jeffrey R.
Husko, Chad A.
Hersam, Mark C.
TI Stable aqueous dispersions of optically and electronically active
phosphorene
SO PROCEEDINGS OF THE NATIONAL ACADEMY OF SCIENCES OF THE UNITED STATES OF
AMERICA
LA English
DT Article
DE black phosphorus; deoxygenated water; liquid phase exfoliation;
photoluminescence; field-effect transistor
ID FIELD-EFFECT TRANSISTORS; EXFOLIATED BLACK PHOSPHORUS; X-RAY
PHOTOELECTRON; SPECTROSCOPY; NANOSHEETS; TRANSPORT; CRYSTALS; GRAPHENE;
MOBILITY
AB Understanding and exploiting the remarkable optical and electronic properties of phosphorene require mass production methods that avoid chemical degradation. Although solution-based strategies have been developed for scalable exfoliation of black phosphorus, these techniques have thus far used anhydrous organic solvents in an effort to minimize exposure to known oxidants, but at the cost of limited exfoliation yield and flake size distribution. Here, we present an alternative phosphorene production method based on surfactant-assisted exfoliation and postprocessing of black phosphorus in deoxygenated water. From comprehensive microscopic and spectroscopic analysis, this approach is shown to yield phosphorene dispersions that are stable, highly concentrated, and comparable to micromechanically exfoliated phosphorene in structure and chemistry. Due to the high exfoliation efficiency of this process, the resulting phosphorene flakes are thinner than anhydrous organic solvent dispersions, thus allowing the observation of layer-dependent photoluminescence down to the monolayer limit. Furthermore, to demonstrate preservation of electronic properties following solution processing, the aqueous-exfoliated phosphorene flakes are used in field-effect transistors with high drive currents and current modulation ratios. Overall, this method enables the isolation and mass production of few-layer phosphorene, which will accelerate ongoing efforts to realize a diverse range of phosphorene-based applications.
C1 [Kang, Joohoon; Wells, Spencer A.; Wood, Joshua D.; Lee, Jae-Hyeok; Ryder, Christopher R.; Zhu, Jian; Hersam, Mark C.] Northwestern Univ, Dept Mat Sci & Engn, Evanston, IL 60208 USA.
[Liu, Xiaolong; Hersam, Mark C.] Northwestern Univ, Grad Program Appl Phys, Evanston, IL 60208 USA.
[Guest, Jeffrey R.; Husko, Chad A.] Argonne Natl Lab, Ctr Nanoscale Mat, 9700 S Cass Ave, Argonne, IL 60439 USA.
[Hersam, Mark C.] Northwestern Univ, Dept Chem, 2145 Sheridan Rd, Evanston, IL 60208 USA.
[Hersam, Mark C.] Northwestern Univ, Dept Med, Evanston, IL 60208 USA.
[Hersam, Mark C.] Northwestern Univ, Dept Elect Engn & Comp Sci, Evanston, IL 60208 USA.
RP Hersam, MC (reprint author), Northwestern Univ, Dept Mat Sci & Engn, Evanston, IL 60208 USA.; Hersam, MC (reprint author), Northwestern Univ, Grad Program Appl Phys, Evanston, IL 60208 USA.; Hersam, MC (reprint author), Northwestern Univ, Dept Chem, 2145 Sheridan Rd, Evanston, IL 60208 USA.; Hersam, MC (reprint author), Northwestern Univ, Dept Med, Evanston, IL 60208 USA.; Hersam, MC (reprint author), Northwestern Univ, Dept Elect Engn & Comp Sci, Evanston, IL 60208 USA.
EM m-hersam@northwestern.edu
RI Guest, Jeffrey/B-2715-2009;
OI Guest, Jeffrey/0000-0002-9756-8801; Liu, Xiaolong/0000-0002-6186-5257
FU National Science Foundation (NSF) [DMR-1505849]; Office of Naval
Research [N00014-14-1-0669]; NSF Materials Research Science and
Engineering Center (MRSEC) Grant [DMR-1121262]; NSF MRSEC Grant
[DMR-1121262]; State of Illinois; Northwestern University;
Argonne-Northwestern Solar Energy Research Energy Frontier Research
Center (Department of Energy) [DE-SC0001059]; US Department of Energy,
Office of Science, Office of Basic Energy Sciences [DE-AC02-06CH11357];
Department of Defense, Air Force Office of Scientific Research, National
Defense Science and Engineering Graduate Fellowship [FA9550-11-C-0028];
Argonne National Laboratory named postdoctoral fellowship
FX We thank D. Jariwala for assistance in measuring black phosphorus
contact angles. Solution processing was supported by National Science
Foundation (NSF) Grant DMR-1505849, structural and chemical
characterization was supported by Office of Naval Research Grant
N00014-14-1-0669, and charge transport measurements were supported by
NSF Materials Research Science and Engineering Center (MRSEC) Grant
DMR-1121262. This work made use of the NUANCE Center, which has received
support from NSF MRSEC Grant DMR-1121262, the State of Illinois, and
Northwestern University. The Raman instrumentation was funded by the
Argonne-Northwestern Solar Energy Research Energy Frontier Research
Center (Department of Energy Grant DE-SC0001059). The use of the
near-infrared microscope at the Argonne National Laboratory Center for
Nanoscale Materials was supported by US Department of Energy, Office of
Science, Office of Basic Energy Sciences Contract DE-AC02-06CH11357.
S.A.W. was supported under Contract FA9550-11-C-0028 from the Department
of Defense, Air Force Office of Scientific Research, National Defense
Science and Engineering Graduate Fellowship. C.A.H. was supported by an
Argonne National Laboratory named postdoctoral fellowship.
NR 33
TC 14
Z9 14
U1 45
U2 45
PU NATL ACAD SCIENCES
PI WASHINGTON
PA 2101 CONSTITUTION AVE NW, WASHINGTON, DC 20418 USA
SN 0027-8424
J9 P NATL ACAD SCI USA
JI Proc. Natl. Acad. Sci. U. S. A.
PD OCT 18
PY 2016
VL 113
IS 42
BP 11688
EP 11693
DI 10.1073/pnas.1602215113
PG 6
WC Multidisciplinary Sciences
SC Science & Technology - Other Topics
GA DZ1PN
UT WOS:000385610400042
PM 27092006
ER
PT J
AU Kawakami, E
Jullien, T
Scarlino, P
Ward, DR
Savage, DE
Lagally, MG
Dobrovitski, VV
Friesen, M
Coppersmith, SN
Eriksson, MA
Vandersypen, LMK
AF Kawakami, Erika
Jullien, Thibaut
Scarlino, Pasquale
Ward, Daniel R.
Savage, Donald E.
Lagally, Max G.
Dobrovitski, Viatcheslav V.
Friesen, Mark
Coppersmith, Susan N.
Eriksson, Mark A.
Vandersypen, Lieven M. K.
TI Gate fidelity and coherence of an electron spin in an Si/SiGe quantum
dot with micromagnet
SO PROCEEDINGS OF THE NATIONAL ACADEMY OF SCIENCES OF THE UNITED STATES OF
AMERICA
LA English
DT Article
DE Si/SiGe quantum dot; qubit; dynamical decoupling; randomized
benchmarking; electron spin
ID SILICON; QUBIT; SECONDS
AB The gate fidelity and the coherence time of a quantum bit (qubit) are important benchmarks for quantum computation. We construct a qubit using a single electron spin in an Si/SiGe quantum dot and control it electrically via an artificial spin-orbit field from a micromagnet. We measure an average single-qubit gate fidelity of similar to 99% using randomized benchmarking, which is consistent with dephasing from the slowly evolving nuclear spins in the substrate. The coherence time measured using dynamical decoupling extends up to similar to 400 mu s for 128 decoupling pulses, with no sign of saturation. We find evidence that the coherence time is limited by noise in the 10-kHz to 1-MHz range, possibly because charge noise affects the spin via the micromagnet gradient. This work shows that an electron spin in an Si/SiGe quantum dot is a good candidate for quantum information processing as well as for a quantum memory, even without isotopic purification.
C1 [Kawakami, Erika; Jullien, Thibaut; Scarlino, Pasquale; Vandersypen, Lieven M. K.] QuTech, NL-2628 CJ Delft, Netherlands.
[Kawakami, Erika; Jullien, Thibaut; Scarlino, Pasquale; Vandersypen, Lieven M. K.] Delft Univ Technol, Kavli Inst Nanosci, NL-2628 CJ Delft, Netherlands.
[Ward, Daniel R.; Savage, Donald E.; Lagally, Max G.; Friesen, Mark; Coppersmith, Susan N.; Eriksson, Mark A.] Univ Wisconsin, Madison, WI 53706 USA.
[Dobrovitski, Viatcheslav V.] Iowa State Univ, US DOE, Ames Lab, Ames, IA 50011 USA.
[Vandersypen, Lieven M. K.] Intel Corp, Components Res, Hillsboro, OR 97124 USA.
RP Vandersypen, LMK (reprint author), QuTech, NL-2628 CJ Delft, Netherlands.; Vandersypen, LMK (reprint author), Delft Univ Technol, Kavli Inst Nanosci, NL-2628 CJ Delft, Netherlands.; Coppersmith, SN (reprint author), Univ Wisconsin, Madison, WI 53706 USA.; Vandersypen, LMK (reprint author), Intel Corp, Components Res, Hillsboro, OR 97124 USA.
EM snc@physics.wisc.edu; l.m.k.vandersypen@tudelft.nl
FU Army Research Office [W911NF-12-0607]; Dutch Foundation for Fundamental
Research on Matter (FOM); European Research Council (ERC) Synergy grant;
Department of Energy (DOE) [DE-FG02-03ER46028]; Nakajima Foundation;
DOE-Basic Energy Sciences [DE-AC02-07CH11358]
FX We acknowledge R. Hanson, G. de Lange, M. Veldhorst, S. Bartlett, and L.
Schreiber for useful discussions, and R. Schouten and R. Vermeulen for
technical support. This work was supported in part by Army Research
Office (W911NF-12-0607), the Dutch Foundation for Fundamental Research
on Matter (FOM), and a European Research Council (ERC) Synergy grant;
development and maintenance of the growth facilities used for
fabricating samples is supported by Department of Energy (DOE)
(DE-FG02-03ER46028). E.K. was supported by a fellowship from the
Nakajima Foundation. This research used National Science
Foundation-supported shared facilities at the University of
Wisconsin-Madison. Work at the Ames Laboratory (analysis of nuclear spin
noise and decoherence) was supported by the DOE-Basic Energy Sciences
under Contract DE-AC02-07CH11358.
NR 40
TC 3
Z9 3
U1 12
U2 12
PU NATL ACAD SCIENCES
PI WASHINGTON
PA 2101 CONSTITUTION AVE NW, WASHINGTON, DC 20418 USA
SN 0027-8424
J9 P NATL ACAD SCI USA
JI Proc. Natl. Acad. Sci. U. S. A.
PD OCT 18
PY 2016
VL 113
IS 42
BP 11738
EP 11743
DI 10.1073/pnas.1603251113
PG 6
WC Multidisciplinary Sciences
SC Science & Technology - Other Topics
GA DZ1PN
UT WOS:000385610400049
PM 27698123
ER
PT J
AU Kornienko, N
Sakimoto, KK
Herlihy, DM
Nguyen, SC
Alivisatos, AP
Harris, CB
Schwartzberg, A
Yang, PD
AF Kornienko, Nikolay
Sakimoto, Kelsey K.
Herlihy, David M.
Nguyen, Son C.
Alivisatos, A. Paul
Harris, Charles. B.
Schwartzberg, Adam
Yang, Peidong
TI Spectroscopic elucidation of energy transfer in hybrid
inorganic-biological organisms for solar-to-chemical production
SO PROCEEDINGS OF THE NATIONAL ACADEMY OF SCIENCES OF THE UNITED STATES OF
AMERICA
LA English
DT Article
DE energy conversion; spectroscopy; CO2 reduction; biohybrid systems;
catalysis
ID ELECTRON-TRANSFER; CLOSTRIDIUM-THERMOACETICUM; ARTIFICIAL
PHOTOSYNTHESIS; ACTIVE-SITE; HYDROGENASE; BACTERIA; CDS; ABSORPTION;
INTERFACES; CONVERSION
AB The rise of inorganic-biological hybrid organisms for solar-to-chemical production has spurred mechanistic investigations into the dynamics of the biotic-abiotic interface to drive the development of next-generation systems. The model system, Moorella thermoacetica-cadmium sulfide (CdS), combines an inorganic semiconductor nanoparticle light harvester with an acetogenic bacterium to drive the photosynthetic reduction of CO2 to acetic acid with high efficiency. In this work, we report insights into this unique electrotrophic behavior and propose a charge-transfer mechanism from CdS to M. thermoacetica. Transient absorption (TA) spectroscopy revealed that photoexcited electron transfer rates increase with increasing hydrogenase (H(2)ase) enzyme activity. On the same time scale as the TA spectroscopy, time-resolved infrared (TRIR) spectroscopy showed spectral changes in the 1,700-1,900-cm(-1) spectral region. The quantum efficiency of this system for photosynthetic acetic acid generation also increased with increasing H(2)ase activity and shorter carrier lifetimes when averaged over the first 24 h of photosynthesis. However, within the initial 3 h of photosynthesis, the rate followed an opposite trend: The bacteria with the lowest H(2)ase activity photosynthesized acetic acid the fastest. These results suggest a two-pathway mechanism: a high quantum efficiency charge-transfer pathway to H(2)ase generating H-2 as a molecular intermediate that dominates at long time scales (24 h), and a direct energy-transducing enzymatic pathway responsible for acetic acid production at short time scales (3 h). This work represents a promising platform to utilize conventional spectroscopic methodology to extract insights from more complex biotic-abiotic hybrid systems.
C1 [Kornienko, Nikolay; Sakimoto, Kelsey K.; Herlihy, David M.; Nguyen, Son C.; Alivisatos, A. Paul; Harris, Charles. B.; Yang, Peidong] Univ Calif Berkeley, Dept Chem, Berkeley, CA 94720 USA.
[Alivisatos, A. Paul; Yang, Peidong] Univ Calif Berkeley, Dept Mat Sci & Engn, Berkeley, CA 94720 USA.
[Alivisatos, A. Paul; Yang, Peidong] Kavli Energy NanoSci Inst, Berkeley, CA 94720 USA.
[Schwartzberg, Adam] Lawrence Berkeley Natl Lab, Mol Foundry, Berkeley, CA 94720 USA.
RP Yang, PD (reprint author), Univ Calif Berkeley, Dept Chem, Berkeley, CA 94720 USA.; Yang, PD (reprint author), Univ Calif Berkeley, Dept Mat Sci & Engn, Berkeley, CA 94720 USA.; Yang, PD (reprint author), Kavli Energy NanoSci Inst, Berkeley, CA 94720 USA.
EM p_yang@berkeley.edu
RI Alivisatos , Paul /N-8863-2015
OI Alivisatos , Paul /0000-0001-6895-9048
FU Office of Science, Office of Basic Energy Sciences, of the US Department
of Energy (DOE) [DE-AC02-05CH11231]; National Science Foundation
[DMR-1507914]; Office of Science, Office of Basic Energy Sciences, of
the US DOE [DE-AC02-05CH11231]
FX This work was supported by the Office of Science, Office of Basic Energy
Sciences, of the US Department of Energy (DOE), under Contract
DE-AC02-05CH11231 (pchem). Solar-to-chemical production experiments were
supported by the National Science Foundation under Grant DMR-1507914. TA
measurements were performed in the Molecular Foundry. Work at the
Molecular Foundry was supported by the Office of Science, Office of
Basic Energy Sciences, of the US DOE under Contract DE-AC02-05CH11231.
NR 41
TC 1
Z9 1
U1 43
U2 43
PU NATL ACAD SCIENCES
PI WASHINGTON
PA 2101 CONSTITUTION AVE NW, WASHINGTON, DC 20418 USA
SN 0027-8424
J9 P NATL ACAD SCI USA
JI Proc. Natl. Acad. Sci. U. S. A.
PD OCT 18
PY 2016
VL 113
IS 42
BP 11750
EP 11755
DI 10.1073/pnas.1610554113
PG 6
WC Multidisciplinary Sciences
SC Science & Technology - Other Topics
GA DZ1PN
UT WOS:000385610400051
PM 27698140
ER
PT J
AU Hu, LF
O'Neil, M
Erturun, V
Benitez, R
Proust, G
Karaman, I
Radovic, M
AF Hu, Liangfa
O'Neil, Morgan
Erturun, Veysel
Benitez, Rogelio
Proust, Gwenaelle
Karaman, Ibrahim
Radovic, Miladin
TI High-Performance Metal/Carbide Composites with Far-From-Equilibrium
Compositions and Controlled Microstructures
SO SCIENTIFIC REPORTS
LA English
DT Article
ID CARBIDE-ALUMINUM COMPOSITES; MATRIX COMPOSITES; MECHANICAL-PROPERTIES;
TENSILE PROPERTIES; MAX PHASES; BEHAVIOR; FRACTURE; INFILTRATION; AL;
REINFORCEMENT
AB The prospect of extending existing metal-ceramic composites to those with the compositions that are far from thermodynamic equilibrium is examined. A current and pressure-assisted, rapid infiltration is proposed to fabricate composites, consisting of reactive metallic and ceramic phases with controlled microstructure and tunable properties. An aluminum (Al) alloy/Ti2AlC composite is selected as an example of the far-from-equilibrium systems to fabricate, because Ti2AlC exists only in a narrow region of the Ti-Al-C phase diagram and readily reacts with Al. This kind of reactive systems challenges conventional methods for successfully processing corresponding metal-ceramic composites. Al alloy/Ti2AlC composites with controlled microstructures, various volume ratios of constituents (40/60 and 27/73) and metallic phase sizes (42-83 mu m, 77-276 mu m, and 167-545 mu m), are obtained using the Ti2AlC foams with different pore structures as preforms for molten metal (Al alloy) infiltration. The resulting composites are lightweight and display exceptional mechanical properties at both ambient and elevated temperatures. These structures achieve a compressive strength that is 10 times higher than the yield strength of the corresponding peak-aged Al alloy at ambient temperature and 14 times higher at 400 degrees C. Possible strengthening mechanisms are described, and further strategies for improving properties of those composites are proposed.
C1 [Hu, Liangfa; Karaman, Ibrahim; Radovic, Miladin] Texas A&M Univ, Dept Mat Sci & Engn, College Stn, TX 77843 USA.
[O'Neil, Morgan; Benitez, Rogelio; Karaman, Ibrahim; Radovic, Miladin] Texas A&M Univ, Dept Mech Engn, College Stn, TX 77843 USA.
[Erturun, Veysel] Erciyes Univ, Dept Airframes & Powerplants, TR-38039 Kayseri, Turkey.
[Proust, Gwenaelle] Univ Sydney, Sch Civil Engn, Sydney, NSW 2006, Australia.
[Hu, Liangfa] US DOE, Ames Lab, Ames, IA 50011 USA.
RP Karaman, I; Radovic, M (reprint author), Texas A&M Univ, Dept Mat Sci & Engn, College Stn, TX 77843 USA.; Karaman, I; Radovic, M (reprint author), Texas A&M Univ, Dept Mech Engn, College Stn, TX 77843 USA.
EM ikaraman@tamu.edu; mradovic@tamu.edu
FU U.S. Air Force Office of Scientific Research; MURI Program
[FA9550-09-10686]; Scientific and Technological Research Council of
Turkey
FX This work was supported by the U.S. Air Force Office of Scientific
Research, MURI Program (FA9550-09-10686) to Texas A&M University. The
authors would like to thank the program manager Dr. David Stargel for
his support. VE would like to thank the Scientific and Technological
Research Council of Turkey for sponsoring his stay at Texas A&M
University. The authors acknowledge the facilities and the scientific
and technical assistance of the Australian Microscopy & Microanalysis
Research Facility at the Australian Centre for Microscopy &
Microanalysis at the University of Sydney, especially Dr. Patrick Trimby
for his assistance with the EBSD characterization and Dr. Matthew Foley
for performing the micro-CT scans.
NR 33
TC 1
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U1 8
U2 8
PU NATURE PUBLISHING GROUP
PI LONDON
PA MACMILLAN BUILDING, 4 CRINAN ST, LONDON N1 9XW, ENGLAND
SN 2045-2322
J9 SCI REP-UK
JI Sci Rep
PD OCT 18
PY 2016
VL 6
AR 35523
DI 10.1038/srep35523
PG 9
WC Multidisciplinary Sciences
SC Science & Technology - Other Topics
GA DZ0BK
UT WOS:000385501900001
PM 27752106
ER
PT J
AU Park, NG
Gratzel, M
Miyasaka, T
Zhu, K
Emery, K
AF Park, Nam-Gyu
Gratzel, Michael
Miyasaka, Tsutomu
Zhu, Kai
Emery, Keith
TI Towards stable and commercially available perovskite solar cells
SO NATURE ENERGY
LA English
DT Article
ID ORGANOMETAL HALIDE PEROVSKITES; CH3NH3PBI3 PEROVSKITE; CHARGE
EXTRACTION; CARBON NANOTUBES; GRAIN-BOUNDARY; BASE ADDUCT; EFFICIENT;
STABILITY; DEGRADATION; IODIDE
AB Solar cells employing a halide perovskite with an organic cation now show power conversion efficiency of up to 22%. However, these cells are facing issues towards commercialization, such as the need to achieve long-term stability and the development of a manufacturing method for the reproducible fabrication of high-performance devices. Here, we propose a strategy to obtain stable and commercially viable perovskite solar cells. A reproducible manufacturing method is suggested, as well as routes to manage grain boundaries and interfacial charge transport. Electroluminescence is regarded as a metric to gauge theoretical efficiency. We highlight how optimizing the design of device architectures is important not only for achieving high efficiency but also for hysteresis-free and stable performance. We argue that reliable device characterization is needed to ensure the advance of this technology towards practical applications. We believe that perovskite-based devices can be competitive with silicon solar modules, and discuss issues related to the safe management of toxic material.
C1 [Park, Nam-Gyu] Sungkyunkwan Univ, Sch Chem Engn, Suwon 440746, South Korea.
[Gratzel, Michael] Ecole Polytech Fed Lausanne, Lab Photon & Interfaces, Inst Chem Sci & Engn, Sch Basic Sci, CH-1015 Lausanne, Switzerland.
[Miyasaka, Tsutomu] Toin Univ Yokohama, Grad Sch Engn, Aoba Ku, Yokohama, Kanagawa 2258503, Japan.
[Zhu, Kai; Emery, Keith] Natl Renewable Energy Lab, Golden, CO 80401 USA.
RP Park, NG (reprint author), Sungkyunkwan Univ, Sch Chem Engn, Suwon 440746, South Korea.
EM npark@skku.edu
RI Park, Nam-Gyu/F-2477-2014
FU National Research Foundation of Korea (NRF) - Ministry of Science, ICT
and Future Planning (MSIP) of Korea [NRF-2012M3A6A7054861,
NRF-2015M1A2A2053004, NRF-2012M3A7B4049986]; US Department of Energy
[DE-AC36-08-GO28308]; National Renewable Energy Laboratory; hybrid
perovskite solar cell program by the US Department of Energy, Office of
Energy Efficiency and Renewable Energy, Solar Energy Technologies
Office; Swiss National Science Foundation (SNSF); NRP 70 'Energy
Turnaround'; SNF-NanoTera; Swiss Federal Office of Energy (SYNERGY);
King Abdulaziz City for Science and Technology (KACST)
FX N.-G.P. acknowledges financial supports from the National Research
Foundation of Korea (NRF) grants funded by the Ministry of Science, ICT
and Future Planning (MSIP) of Korea under contracts No.
NRF-2012M3A6A7054861 (Global Frontier R&D Program on Center for
Multiscale Energy System), NRF-2015M1A2A2053004 (Climate Change
Management Program), and NRF-2012M3A7B4049986 (Nano Material Technology
Development Program). T.M. thanks Japan Science and Technology Agency
(JST) Advanced Low Carbon Technology R&D Program (ALCA) and NEDO
research projects. The NREL portion of this work was supported by the US
Department of Energy under Contract No. DE-AC36-08-GO28308 with the
National Renewable Energy Laboratory. K.Z. acknowledges support by the
hybrid perovskite solar cell program by the US Department of Energy,
Office of Energy Efficiency and Renewable Energy, Solar Energy
Technologies Office. M.G. acknowledges financial support from the Swiss
National Science Foundation (SNSF), the NRP 70 'Energy Turnaround' as
well as from SNF-NanoTera and Swiss Federal Office of Energy (SYNERGY).
He thanks the King Abdulaziz City for Science and Technology (KACST) for
financial support under a joint research project. He also thanks G.
Rothenberger for his help with the kinetic analysis and the drawings
presented in Fig. 2. M.G. acknowledges his affiliation as a visiting
faculty member with Nanyang Technical University (NTU) Singapore and
Sungkyunkwan University (SKKU) Seoul Korea.
NR 51
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U1 12
U2 12
PU NATURE PUBLISHING GROUP
PI LONDON
PA MACMILLAN BUILDING, 4 CRINAN ST, LONDON N1 9XW, ENGLAND
SN 2058-7546
J9 NAT ENERGY
JI Nat. Energy
PD OCT 17
PY 2016
VL 1
AR 16152
DI 10.1038/NENERGY.2016.152
PG 8
WC Energy & Fuels; Materials Science, Multidisciplinary
SC Energy & Fuels; Materials Science
GA EL7HH
UT WOS:000394791200001
ER
PT J
AU Agbo, P
Abergel, RJ
AF Agbo, Peter
Abergel, Rebecca J.
TI Ligand-Sensitized Lanthanide Nanocrystals: Merging Solid-State
Photophysics and Molecular Solution Chemistry
SO INORGANIC CHEMISTRY
LA English
DT Article
ID UP-CONVERSION; ENERGY-TRANSFER; DOWNCONVERSION LUMINESCENCE; BIOIMAGING
APPLICATIONS; OPTICAL-PROPERTIES; D-BLOCK; COMPLEXES; NANOPARTICLES;
IONS; EMISSION
AB To date, the breadth of scientific research that has been devoted to investigating the photochemical and photophysical behavior of the lanthanide elements has generally fallen into one of two camps: solution studies of luminescent lanthanide metal ligand complexes or investigations of solid-state nanoparticles, composed primarily of, or doped with, lanthanide lumiphores. In the latter case, most research of lanthanide nanocolloids has precluded any investigations regarding the use of organic ligands to overcome the difficulties associated with f-f excitation of lanthanides. Instead, most work on condensed-phase lanthanide luminescence has centered on strategies such as d-f charge separation in divalent lanthanides and the sensitization of lanthanide excited states using quantum dots. Current work now aims at bridging the camps of condensed-phase lanthanide photophysics and the solution chemistry of ligand lanthanide molecular complexes. Recent efforts have partly focused on the fundamental characterization of NaGd(1-x)Ln(x)F(4) nanoparticles featuring surface display of the sensitizer ligand 3,4,3-LI(1,2-HOPO), showing these structures to be capable of converting absorbed UV light into luminescence from Eu3+ and Tb3+ ions. These results suggest such a use of the ligand sensitization as a tool of choice to overcome the constraints of UV solar spectrum/semiconductor band-gap mismatch and low absorption cross sections in solid-state lanthanide systems.
C1 [Agbo, Peter; Abergel, Rebecca J.] Lawrence Berkeley Natl Lab, Div Chem Sci, Berkeley, CA 94720 USA.
RP Abergel, RJ (reprint author), Lawrence Berkeley Natl Lab, Div Chem Sci, Berkeley, CA 94720 USA.
EM rjabergel@lbl.gov
FU U.S. Department of Energy, Office of Science, Office of Basic Energy
Sciences, Chemical Sciences, Geosciences, and Biosciences Division at
the Lawrence Berkeley National Laboratory [DE-AC02-05CH11231]; U.S.
Department of Energy, Office of Science, Early Career Award
FX We thank Dr. Joseph Pacold for his helpful insights regarding internal
quantum yield determination and Tao Xu for his help with TEM imaging.
This work was supported by the U.S. Department of Energy, Office of
Science, Office of Basic Energy Sciences, Chemical Sciences,
Geosciences, and Biosciences Division, at the Lawrence Berkeley National
Laboratory under Contract DE-AC02-05CH11231. R.J.A. is the recipient of
a U.S. Department of Energy, Office of Science, Early Career Award.
NR 76
TC 3
Z9 3
U1 17
U2 17
PU AMER CHEMICAL SOC
PI WASHINGTON
PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA
SN 0020-1669
EI 1520-510X
J9 INORG CHEM
JI Inorg. Chem.
PD OCT 17
PY 2016
VL 55
IS 20
BP 9973
EP 9980
DI 10.1021/acs.inorgchem.6b00879
PG 8
WC Chemistry, Inorganic & Nuclear
SC Chemistry
GA DZ3YL
UT WOS:000385785700004
PM 27362470
ER
PT J
AU Pham, TA
Altman, AB
Stieber, SCE
Booth, CH
Kozimor, SA
Lukens, WW
Olive, DT
Tyliszczak, T
Wang, J
Minasian, SG
Raymond, KN
AF Pham, Tiffany A.
Altman, Alison B.
Stieber, S. Chantal E.
Booth, Corwin H.
Kozimor, Stosh A.
Lukens, Wayne W.
Olive, Daniel T.
Tyliszczak, Tolek
Wang, Jian
Minasian, Stefan G.
Raymond, Kenneth N.
TI A Macrocyclic Chelator That Selectively Binds Ln(4+) over Ln(3+) by a
Factor of 10(29)
SO INORGANIC CHEMISTRY
LA English
DT Article
ID X-RAY-ABSORPTION; CORE-LEVEL SPECTROSCOPY; RARE-EARTH-OXIDES; OXYGEN
K-EDGE; NONCLASSICAL ORGANOLANTHANIDE CHEMISTRY; RESONANT
AUGER-SPECTROSCOPY; CERIUM(IV) AMMONIUM-NITRATE;
SLOW-MAGNETIC-RELAXATION; ADVANCED LIGHT-SOURCE; ELECTRONIC-STRUCTURE
AB A tetravalent cerium macrocyclic complex (CeLK4) was prepared with an octadentate terephthalamide ligand comprised of hard catecholate donors and characterized in the solution state by spectrophotometric titrations and electrochemistry and in the crystal by X-ray diffraction. The solution-state studies showed that L exhibits a remarkably high affinity toward Ce4+, with log beta(110) = 61(2) and Delta G = -348 kJ/mol, compared with log beta(110) = 32.02(2) for the analogous Pr3+ complex. In addition, L exhibits an unusual preference for forming CeL4- relative to formation of the analogous actinide complex, ThL4-, which has beta(110) = 53.7(5). The extreme stabilization of tetravalent cerium relative to its trivalent state is also evidenced by the shift of 1.91 V in the redox potential of the Ce3+/Ce4+ couple of the complex (measured at -0.454 V vs SHE). The unprecedented behavior prompted an electronic structure analysis using L-3- and M-5,M-4-edge X-ray absorption near-edge structure (XANES) spectroscopies and configuration interaction calculations, which showed that 4f-orbital bonding in CeLK4 has partial covalent character due to ligand-to-metal charge transfer (LMCT) in the ground state. The experimental results are presented in the context of earlier measurements on tetravalent cerium compounds, indicating that the amount of LMCT for CeLK4 is similar to that observed for [Et4N](2)[CeCl6] and CeO2 and significantly less than that for the organometallic sandwich compound cerocene, (C8H8)(2)Ce. A simple model to rationalize changes in 4f orbital bonding for tri- and tetravalent lanthanide and actinide compounds is also provided.
C1 [Pham, Tiffany A.; Altman, Alison B.; Raymond, Kenneth N.] Univ Calif Berkeley, Berkeley, CA 94720 USA.
[Pham, Tiffany A.; Altman, Alison B.; Booth, Corwin H.; Lukens, Wayne W.; Olive, Daniel T.; Tyliszczak, Tolek; Minasian, Stefan G.; Raymond, Kenneth N.] LBNL, Berkeley, CA 94720 USA.
[Stieber, S. Chantal E.; Kozimor, Stosh A.] LANL, Los Alamos, NM 87545 USA.
[Stieber, S. Chantal E.] Calif State Polytech Univ Pomona, Pomona, CA 91768 USA.
[Wang, Jian] CLS, Saskatoon, SK S7N 2V3, Canada.
RP Raymond, KN (reprint author), Univ Calif Berkeley, Berkeley, CA 94720 USA.; Minasian, SG; Raymond, KN (reprint author), LBNL, Berkeley, CA 94720 USA.
EM sgminasian@lbl.gov; raymond@socrates.berkeley.edu
FU Office of Science, Office of Basic Energy Sciences, Division of Chemical
Sciences, Geosciences, and Biosciences, Heavy Element Chemistry Program
of the U.S. Department of Energy (DOE) [DE-AC02-05CH11231]; University
of California, Berkeley; U.S. DOE Integrated University Program
Fellowship; Office of Science, Office of Basic Energy Sciences, Division
of Chemical Sciences, Geosciences, and Biosciences, Heavy Element
Chemistry Program of the U.S. DOE; National Nuclear Security
Administration of the U.S. DOE [DE-AC52-06NA25396]; Glenn T. Seaborg
Institute Postdoctoral Fellowship; College of Science; Office of
Science, Office of Basic Energy Sciences, Division of Chemical Sciences,
Geosciences, and Biosciences Condensed Phase and Interfacial Molecular
Sciences Program of the U.S. DOE [DE-AC02-05CH11231]; U.S. DOE, Office
of Science, Office of Basic Energy Sciences [DE-AC02-76SF00515]; Canada
Foundation for Innovation; Natural Sciences and Engineering Research
Council of Canada; University of Saskatchewan; Government of
Saskatchewan; Western Economic Diversification Canada; National Research
Council Canada; Canadian Institutes of Health Research; Office of
Science, Office of Basic Energy Sciences, of the U.S. DOE
[DE-AC02-05CH11231]
FX The authors thank Drs. Michael Nippe and David Tatum for their
invaluable help with electrochemical and NMR experiments, respectively.
C.H.B., W.W.L., S.G.M., D.T.O., and K.N.R. were supported at LBNL by the
Director, Office of Science, Office of Basic Energy Sciences, Division
of Chemical Sciences, Geosciences, and Biosciences, Heavy Element
Chemistry Program of the U.S. Department of Energy (DOE) under Contract
DE-AC02-05CH11231. S.A.K. and C.E.S. were supported at LANL by the
Director, Office of Science, Office of Basic Energy Sciences, Division
of Chemical Sciences, Geosciences, and Biosciences, Heavy Element
Chemistry Program of the U.S. DOE. LANL is operated by Los Alamos
National Security, LLC, for the National Nuclear Security Administration
of the U.S. DOE under Contract DE-AC52-06NA25396. Portions of this work
were supported at the University of California, Berkeley, by a U.S. DOE
Integrated University Program Fellowship (to A.B.A.), at LANL by a Glenn
T. Seaborg Institute Postdoctoral Fellowship (to C.E.S.), and at the
California State Polytechnic University, Pomona by the College of
Science (to C.E.S.). Research described in this paper was also performed
at the CLS, which is supported by the Canada Foundation for Innovation,
Natural Sciences and Engineering Research Council of Canada, the
University of Saskatchewan, the Government of Saskatchewan, Western
Economic Diversification Canada, the National Research Council Canada,
and the Canadian Institutes of Health Research. T.T. and the ALS were
supported at LBNL by the Director, Office of Science, Office of Basic
Energy Sciences, of the U.S. DOE under Contract DE-AC02-05CH11231.
Research at Beamline 11.0.2 at the ALS was supported at LBNL by the
Director, Office of Science, Office of Basic Energy Sciences, Division
of Chemical Sciences, Geosciences, and Biosciences Condensed Phase and
Interfacial Molecular Sciences Program of the U.S. DOE under Contract
DE-AC02-05CH11231. Use of the Stanford Synchrotron Radiation
Lightsource, SLAC National Accelerator Laboratory, is supported by the
U.S. DOE, Office of Science, Office of Basic Energy Sciences, under
Contract DE-AC02-76SF00515.
NR 178
TC 1
Z9 1
U1 11
U2 11
PU AMER CHEMICAL SOC
PI WASHINGTON
PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA
SN 0020-1669
EI 1520-510X
J9 INORG CHEM
JI Inorg. Chem.
PD OCT 17
PY 2016
VL 55
IS 20
BP 9989
EP 10002
DI 10.1021/acs.inorgchem.6b00684
PG 14
WC Chemistry, Inorganic & Nuclear
SC Chemistry
GA DZ3YL
UT WOS:000385785700006
PM 27341328
ER
PT J
AU Lin, J
Jin, GB
Soderholm, L
AF Lin, Jian
Jin, Geng Bang
Soderholm, L.
TI Th-3[Th-6(OH)(4)O-4(H2O)(6)](SO4)(12)(H2O)(13): A Self-Assembled
Microporous Open-Framework Thorium Sulfate
SO INORGANIC CHEMISTRY
LA English
DT Article
ID METAL-ORGANIC FRAMEWORKS; CRYSTAL-STRUCTURE; AQUEOUS-SOLUTION;
COORDINATION POLYMERS; MOLECULAR CLUSTERS; HEXANUCLEAR; CHEMISTRY; CORE;
COMPLEX; SPECIATION
AB A neutral-framework thorium oxohydroxosulfate hydrate has been isolated from aqueous solution. This microporous structure, which self-assembles without a templating agent, is built from [Th-6(OH)(4)O-4(H2O)(6)](12+) hexamers and thorium(IV) monomers linked through bridging sulfates. Solution conditions were chosen to enable an active competition between sulfate and hydroxide for thorium coordination. Synthetic requirements are discussed for this rare example of a thorium(IV) polynuclear complex containing mixed oxo-, hydroxo-, and sulfato-bridging moieties.
C1 [Lin, Jian; Jin, Geng Bang; Soderholm, L.] Argonne Natl Lab, Chem Sci & Engn Div, Argonne, IL 60439 USA.
RP Jin, GB; Soderholm, L (reprint author), Argonne Natl Lab, Chem Sci & Engn Div, Argonne, IL 60439 USA.
EM GJin@anl.gov; ls@anl.gov
FU U.S. DOE BES Heavy Elements Program [DE-AC0206CH11357]
FX The work is supported by the U.S. DOE BES Heavy Elements Program under
Contract DE-AC0206CH11357.
NR 46
TC 0
Z9 0
U1 6
U2 6
PU AMER CHEMICAL SOC
PI WASHINGTON
PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA
SN 0020-1669
EI 1520-510X
J9 INORG CHEM
JI Inorg. Chem.
PD OCT 17
PY 2016
VL 55
IS 20
BP 10098
EP 10101
DI 10.1021/acs.inorgchem.6b01762
PG 4
WC Chemistry, Inorganic & Nuclear
SC Chemistry
GA DZ3YL
UT WOS:000385785700018
PM 27665624
ER
PT J
AU Li, MR
Deng, Z
Lapidus, SH
Stephens, PW
Segre, CU
Croft, M
Sena, RP
Hadermann, J
Walker, D
Greenblatt, M
AF Li, Man-Rong
Deng, Zheng
Lapidus, Saul H.
Stephens, Peter W.
Segre, Carlo U.
Croft, Mark
Sena, Robert Paria
Hadermann, Joke
Walker, David
Greenblatt, Martha
TI Ba-3(Cr0.97(1)Te0.03(1))(2)TeO9: in Search of Jahn-Teller Distorted
Cr(II) Oxide
SO INORGANIC CHEMISTRY
LA English
DT Article
ID HIGH-TEMPERATURE SUPERCONDUCTIVITY; CRYSTAL-STRUCTURE;
MAGNETIC-PROPERTIES; DOUBLE PEROVSKITE; HIGH-PRESSURE; CHARGE
DISPROPORTIONATION; A-SITE; LA; PHASE; ND
AB A novel 6H-type hexagonal perovskite Ba-3(Cr0.97(1)Te0.03(1))(2)TeO9 was prepared at high pressure (6 GPa) and temperature (1773 K). Both transmission electron microscopy and synchrotron powder X-ray diffraction data demonstrate that Ba-3(Cr0.97(1)Te0.03(1))(2)TeO9 crystallizes in P6(3)/mmc with face-shared (Cr0.97(1)Te0.03(1))O-6 octahedral pairs interconnected with TeO6 octahedra via corner-sharing. Structure analysis shows a mixed Cr2+/Cr3+ valence state with similar to 10% Cr2+. The existence of Cr2+ in Ba-3(Cr0.10(1)2+Cr0.87(1)3+Te0.036+)(2)TeO9 is further evidenced by X-ray absorption near-edge spectroscopy. Magnetic properties measurements show a paramagnetic response down to 4 K and a small glassy-state curvature at low temperature. In this work, the octahedral Cr2+O6 component is stabilized in an oxide material for the first time; the expected Jahn-Teller distortion of high-spin (d(4)) Cr2+ is not found, which is attributed to the small proportion of Cr2+ (similar to 10%) and the face-sharing arrangement of CrO6 octahedral pairs, which structurally disfavor axial distortion.
C1 [Li, Man-Rong; Deng, Zheng; Greenblatt, Martha] Rutgers State Univ, Dept Chem & Chem Biol, 610 Taylor Rd, Piscataway, NJ 08854 USA.
[Lapidus, Saul H.] Argonne Natl Lab, Adv Photon Source, Lemont, IL 60439 USA.
[Stephens, Peter W.] SUNY Stony Brook, Dept Phys & Astron, Stony Brook, NY 11794 USA.
[Segre, Carlo U.] IIT, Dept Phys, 3300 South Fed St, Chicago, IL 60616 USA.
[Segre, Carlo U.] IIT, CSRRI, 3300 South Fed St, Chicago, IL 60616 USA.
[Croft, Mark] Rutgers State Univ, Dept Phys & Astron, 136 Frelinghusen Rd, Piscataway, NJ 08854 USA.
[Sena, Robert Paria; Hadermann, Joke] Univ Antwerp, EMAT, Groenenborgerlaan 171, B-2020 Antwerp, Belgium.
[Walker, David] Columbia Univ, Lamont Doherty Earth Observ, 61 Route 9W,POB 1000, Palisades, NY 10964 USA.
RP Greenblatt, M (reprint author), Rutgers State Univ, Dept Chem & Chem Biol, 610 Taylor Rd, Piscataway, NJ 08854 USA.
EM martha@rutchem.rutgers.edu
RI Segre, Carlo/B-1548-2009; ID, MRCAT/G-7586-2011; Hadermann,
Joke/F-4644-2011
OI Segre, Carlo/0000-0001-7664-1574;
FU Department of Energy; MRCAT; U.S. Department of Energy
[DE-AC02-06CH11357]; [NSF-DMR-1507252]
FX This work was supported by the NSF-DMR-1507252 grant. MRCAT operations
are supported by the Department of Energy and the MRCAT member
institutions. Use of the Argonne National Laboratory and the Advanced
Photon Source is supported by the U.S. Department of Energy, under
Contract No. DE-AC02-06CH11357. The authors would like to thank Dr. S.
W. Kim at Rutgers Univ. for making a precursor, Ms. J. Hanley at LDEO in
Columbia Univ. for making the high-pressure assemblies, and Dr. A. Fiege
at the American Museum of Natural History in New York City for the
assistance of microprobe analyses.
NR 65
TC 0
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U1 6
U2 6
PU AMER CHEMICAL SOC
PI WASHINGTON
PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA
SN 0020-1669
EI 1520-510X
J9 INORG CHEM
JI Inorg. Chem.
PD OCT 17
PY 2016
VL 55
IS 20
BP 10135
EP 10142
DI 10.1021/acs.inorgchem.6b01047
PG 8
WC Chemistry, Inorganic & Nuclear
SC Chemistry
GA DZ3YL
UT WOS:000385785700026
PM 27680715
ER
PT J
AU Kim, SW
Deng, Z
Fischer, Z
Lapidus, SH
Stephens, PW
Li, MR
Greenblatt, M
AF Kim, Sun Woo
Deng, Zheng
Fischer, Zachary
Lapidus, Saul H.
Stephens, Peter W.
Li, Man-Rong
Greenblatt, Martha
TI Structure and Magnetic Behavior of Layered Honeycomb Tellurates,
BiM(III)TeO6 (M = Cr, Mn, Fe)
SO INORGANIC CHEMISTRY
LA English
DT Article
ID CRYSTAL-STRUCTURE; LATTICE; SPIN; NI; IRIDATE; PBSB2O6; SERIES; CO
AB New layered honeycomb tellurates, BiM(III)-TeO6 (M = Cr, Mn, Fe) were synthesized and characterized. BiM(III)TeO6 (M = Cr, Fe) species crystallize in a trigonal space group, P (3) over bar 1c (No. 163), of edge-sharing M3+/Te6+O6 octahedra, which form honeycomb-like double layers in the ab plane with Bi3+ cations located between the layers. Interestingly, the structure of BiMnTeO6 is similar to those of the Cr/Fe analogues, but with monoclinic space group, P2(1)/c (No. 14), attributed to the strong Jahn-Teller distortion of Mn3+ cations. The crystal structure of BiM(III)TeO6 is a superstructure of PbSb2O6-related materials (ABB'O-6). The Cr3+ and Fe3+ cations are ordered 80% and 90%, respectively, while the Mn3+ ions are completely ordered on the B-site of the ABB'O-6 structure. BiCrTeO6 shows a broad antiferromagnetic transition (AFM) at similar to 17 K with a Weiss temperature (theta) of -59.85 K, while BiFeTeO6 and BiMnTeO6 show sharp AFM transitions at similar to 11 K with theta of -27.56 K and at similar to 9.5 K with theta of -17.57 K, respectively. These differences in the magnetic behavior are ascribed to the different concentration of magnetic nearest versus next-nearest neighbor interactions of magnetic cations due to the relative differences in the extent of M/Te ordering.
C1 [Kim, Sun Woo; Deng, Zheng; Fischer, Zachary; Li, Man-Rong; Greenblatt, Martha] Rutgers State Univ, Dept Chem & Chem Biol, 610 Taylor Rd, Piscataway, NJ 08854 USA.
[Lapidus, Saul H.] Argonne Natl Lab, Adv Photon Source, Lemont, IL 60439 USA.
[Stephens, Peter W.] SUNY Stony Brook, Dept Phys & Astron, Stony Brook, NY 11794 USA.
RP Greenblatt, M (reprint author), Rutgers State Univ, Dept Chem & Chem Biol, 610 Taylor Rd, Piscataway, NJ 08854 USA.
EM martha@chem.rutgers.edu
FU DOE Office of Science by Argonne National Laboratory
[DE-AC02-06CH11357]; [NSF-DMR-1507252]
FX S.W.K., Z.D., Z.F., M.-R.L., and M.G. gratefully acknowledge support
from NSF-DMR-1507252 grant. This research used resources of the Advanced
Photon Source, a U.S. Department of Energy (DOE) Office of Science User
Facility operated for the DOE Office of Science by Argonne National
Laboratory under Contract DE-AC02-06CH11357.
NR 40
TC 0
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U2 9
PU AMER CHEMICAL SOC
PI WASHINGTON
PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA
SN 0020-1669
EI 1520-510X
J9 INORG CHEM
JI Inorg. Chem.
PD OCT 17
PY 2016
VL 55
IS 20
BP 10229
EP 10237
DI 10.1021/acs.inorgchem.6b01472
PG 9
WC Chemistry, Inorganic & Nuclear
SC Chemistry
GA DZ3YL
UT WOS:000385785700036
PM 27676324
ER
PT J
AU Wang, Q
Liao, XY
Xu, WQ
Ren, Y
Livi, KJ
Zhu, MQ
AF Wang, Qian
Liao, Xianya
Xu, Wenqian
Ren, Yang
Livi, Kenneth J.
Zhu, Mengqiang
TI Synthesis of Birnessite in the Presence of Phosphate, Silicate, or
Sulfate
SO INORGANIC CHEMISTRY
LA English
DT Article
ID WATER-OXIDATION CATALYSIS; BIOGENIC MN-OXIDES; MANGANESE OXIDES;
PARTICLE-SIZE; CRYSTAL-STRUCTURES; LAYER STRUCTURE; ADSORPTION;
SORPTION; MN(III); DIOXIDE
AB Layered manganese (Mn) oxides, such as birnessite, are versatile materials in industrial applications and common minerals mediating elemental cycling in natural environment. Many of birnessite properties are controlled by Mn(III) concentration and particle sizes. Thus, it is important to synthesize birnessite nanoparticles with controlled Mn(III) concentrations and sizes so that one can tune its properties for many applications. Birnessite was synthesized in the presence of oxyanions (phosphate, silicate, or sulfate) during reductive precipitation of KMnO4 by HO. and characterized using multiple synchrotron X-ray techniques, electron microscopy, and diffuse reflectance UV vis spectroscopy. Results indicate that all three anions decrease MnO6 sheet sizes, attributed to oxyanion adsorption on edges of the sheets, inhibiting their lateral growth. As a result of decreased sizes, sheets undergo significant structural contraction. Meanwhile, Mn(III) concentration significantly increases with increasing oxyanion/Mn ratio. The increased Mn(III) concentration, along with the decreased size, enlarges both direct and indirect band gaps of birnessite. Phosphate imposes the strongest influence, followed by silicate and then by sulfate, consistent with their decreasing adsorption affinity. Reacting with 1 M KOH solution effectively removed the adsorbed oxyanions while leading to increased sheet sizes, probably due to oriented attachment-driven particle growth mechanisms. The results have important implications for developing highly performed birnessite materials, for example, small size Mn(III)-rich birnessite for photochemical and catalytic applications, as well as for understanding chemical compositional variations of naturally occurring birnessite.
C1 [Wang, Qian; Liao, Xianya; Zhu, Mengqiang] Univ Wyoming, Dept Ecosyst Sci & Management, Laramie, WY 82071 USA.
[Xu, Wenqian] Brookhaven Natl Lab, Dept Chem, Upton, NY 11973 USA.
[Ren, Yang] Argonne Natl Lab, Xray Sci Div, Adv Photon Source, Argonne, IL 60439 USA.
[Livi, Kenneth J.] Johns Hopkins Univ, Dept Mat Sci & Engn, Mat Characterizat & Proc Ctr, Baltimore, MD 21218 USA.
RP Zhu, MQ (reprint author), Univ Wyoming, Dept Ecosyst Sci & Management, Laramie, WY 82071 USA.
EM mzhu6@uwyo.edu
FU U.S. National Science Foundation [EAR-1529937]; Wyoming Reclamation and
Restoration Center at the Univ. of Wyoming; DOE Office of Science by
Argonne National Laboratory [DE-AC02-06CH11357]; U.S. DOE, Office of
Science, Office of Basic Energy Sciences [DE-AC02-76SF00515]
FX This work was supported by the U.S. National Science Foundation under
Grant No. EAR-1529937 and the Wyoming Reclamation and Restoration Center
at the Univ. of Wyoming. We acknowledge Prof. B. A. Parkinson at the
Dept. of Chemistry, Univ. of Wyoming, for his help with UV-vis diffuse
reflectance spectra collection. We thank beamline scientists K. W.
Chapman, K. A. Beyer, and O. J. Borkiewicz at beamline 11 ID-B and M. G.
Newville and A. Lanzirotti at beamline 13-ID-E at the Advanced Photon
Source (APS), and E. J. Nelson and M. J. Latimer at beamline 14-3 at the
Stanford Synchrotron Radiation Lightsource (SSRL) for their technical
assistance in data collection. This research used resources of the APS,
a U.S. Department of Energy (DOE) Office of Science User Facility
operated for the DOE Office of Science by Argonne National Laboratory
under Contract No. DE-AC02-06CH11357. Use of the SSRL, SLAC National
Accelerator Laboratory, is supported by the U.S. DOE, Office of Science,
Office of Basic Energy Sciences, under Contract No. DE-AC02-76SF00515.
NR 77
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PI WASHINGTON
PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA
SN 0020-1669
EI 1520-510X
J9 INORG CHEM
JI Inorg. Chem.
PD OCT 17
PY 2016
VL 55
IS 20
BP 10248
EP 10258
DI 10.1021/acs.inorgchem.6b01465
PG 11
WC Chemistry, Inorganic & Nuclear
SC Chemistry
GA DZ3YL
UT WOS:000385785700038
PM 27672696
ER
PT J
AU Pham, J
Kreyssig, A
Goldman, AI
Miller, GJ
AF Pham, Joyce
Kreyssig, Andreas
Goldman, Alan I.
Miller, Gordon J.
TI An Icosahedral Quasicrystal and Its 1/0 Crystalline Approximant in the
Ca-Au-Al System
SO INORGANIC CHEMISTRY
LA English
DT Article
ID ELECTRONIC-STRUCTURE; INTERMETALLIC COMPOUNDS; PERIODIC CRYSTALS; CUBIC
APPROXIMANT; CRYSTALLOGRAPHY; ALLOYS; PHASES; CELL; YB; VISUALIZATION
AB A new icosahedral quasicrystalline phase, CaAu4.5-xAl1.5+x [0.11 <= x <= 0.40(6); CaAu4.4Al1.6, a(QC) = 5.383(4) angstrom, and Pm (3) over bar(5) over bar], and its lowest-order 1/0 cubic crystalline approximant phase, CaAu3+xAl1-x [0 <= x <= 0.31(1); a = 9.0766(5)-9.1261(8) angstrom, Pa (3) over bar (No. 205), and Pearson symbol cP40], have been discovered in the Ca-poor region of the Ca-Au-Al system. In the crystalline approximant, eight [Au3-xAl1+x] tetrahedra fill the unit cell, and each tetrahedron is surrounded by four Ca atoms, thus forming a three-dimensional network of {Ca-4/4[Au3-xAl1+x]} tetrahedral stars. A computational study of Au and Al site preferences concurs with the experimental results, which indicate a preference for near-neighbor Au-Al interactions over Au-Au and Al-Al interactions. Analysis of the electronic density of states and the associated crystal orbital Hamilton population curves was used to rationalize the descriptions of CaAu4.5-xAl1.5+x [0.11 <= x <= 0.46(6)] and CaAu3+xAl1-x [0 <= x <= 0.31(1)] as polar intermetallic species, whereby Ca atoms engage in polar covalent bonding with the electronegative, electron-deficient [Au3-xAl1+x] tetrahedral clusters and the observed phase width of the crystalline approximant.
C1 [Pham, Joyce; Miller, Gordon J.] Iowa State Univ, Dept Chem, Ames, IA 50011 USA.
[Kreyssig, Andreas; Goldman, Alan I.] Iowa State Univ, Dept Phys, Ames, IA 50011 USA.
[Pham, Joyce; Kreyssig, Andreas; Goldman, Alan I.; Miller, Gordon J.] Ames Lab, Ames, IA 50011 USA.
RP Miller, GJ (reprint author), Iowa State Univ, Dept Chem, Ames, IA 50011 USA.; Miller, GJ (reprint author), Ames Lab, Ames, IA 50011 USA.
EM gmiller@iastate.edu
FU U.S. National Science Foundation [DMR 10-05765]; Office of the Basic
Energy Sciences, Materials Sciences Division, U.S. Department of Energy
(DOE), at Ames Laboratory; DOE by Iowa State University
[DE-AC02-07CH11358]; U.S. DOE [DE-AC02-06CH11357]; Iowa State University
Computation Advisory Committee Project [202-17-10-08-0005]
FX J.P. acknowledges J. Grin, Q Lin, L. Lutz-Kappelman, V. Smetana, S.
Thimmaiah, and Y. Zhang for fruitful discussions and also thanks S.
Saunders and B. Ueland for assistance with data collection at the
Argonne National Laboratory, S. Bud'ko for resistivity measurements, and
W. Straszheim for EDS measurements. The authors also thank the reviewers
for useful comments. This research was largely supported by the U.S.
National Science Foundation via Grant DMR 10-05765. Diffraction
instrumentation was provided by support of the Office of the Basic
Energy Sciences, Materials Sciences Division, U.S. Department of Energy
(DOE), at Ames Laboratory. Ames Laboratory is operated for DOE by Iowa
State University under Contract DE-AC02-07CH11358. High-energy
diffraction experiments were operated at the APS at the Argonne National
Laboratory (beamline 6ID-D) under the U.S. DOE under Contract
DE-AC02-06CH11357. The computations were done on the CRUNCH system
supported by Iowa State University Computation Advisory Committee
Project 202-17-10-08-0005.
NR 83
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PU AMER CHEMICAL SOC
PI WASHINGTON
PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA
SN 0020-1669
EI 1520-510X
J9 INORG CHEM
JI Inorg. Chem.
PD OCT 17
PY 2016
VL 55
IS 20
BP 10425
EP 10437
DI 10.1021/acs.inorgchem.6b01636
PG 13
WC Chemistry, Inorganic & Nuclear
SC Chemistry
GA DZ3YL
UT WOS:000385785700057
PM 27682453
ER
PT J
AU Childs, BC
Braband, H
Lawler, K
Mast, DS
Bigler, L
Stalder, U
Forster, PM
Czerwinski, KR
Alberto, R
Sattelberger, AP
Poineau, F
AF Childs, Bradley C.
Braband, Henrik
Lawler, Keith
Mast, Daniel S.
Bigler, Laurent
Stalder, Urs
Forster, Paul M.
Czerwinski, Kenneth R.
Alberto, Roger
Sattelberger, Alfred P.
Poineau, Frederic
TI Ditechnetium Heptoxide Revisited: Solid-State, Gas-Phase, and
Theoretical Studies
SO INORGANIC CHEMISTRY
LA English
DT Article
ID GAUSSIAN-BASIS SETS; TECHNETIUM HEPTOXIDE; CRYSTAL-STRUCTURE; DFT
CALCULATIONS; OXIDE; RHENIUM; METAL; OXIDATION; CATALYSTS; STRESS
AB Ditechnetium heptoxide was synthesized from the oxidation of TcO2 with O-2 at 450 degrees C and characterized by single-crystal X-ray diffraction, electron-impact mass spectrometry (EI-MS), and theoretical methods. Refinement of the structure at 100 K indicates that Tc2O7 crystallizes as a molecular solid in the orthorhombic space group Pbca [a = 7.312(3) angstrom, b = 5.562(2) angstrom, c = 13.707(5) angstrom, and V = 557.5(3) angstrom(3)]. The Tc2O7 molecule can be described as corner-sharing TcO4 tetrahedron [Tc---Tc = 3.698(1) angstrom and Tc-O-Bri-Tc = 180.0 degrees]. The EI-MS spectrum of Tc2O7 consists of both mononuclear and dinuclear species. The main dinuclear species in the gas-phase are Tc2O7 (100%) and Tc2O5 (56%), while the main mononuclear species are TcO3 (33.9%) and TcO2 (42.8%). The difference in the relative intensities of the M2O5 (M = Tc, Re) fragments (1.7% for Re) indicates that these group 7 elements exhibit different gas-phase chemistry. The solid-state structure of Tc2O7 was investigated by density functional theory methods. The optimized structure of the Tc2O7 molecule is in good agreement with the experimental one. Simulations indicate that the more favorable geometry for the Tc2O7 molecule in the gas-phase is bent (Tc-O-Bri-Tc = 156.5 degrees), while a linear geometry (Tc-O-Bri-Tc = 180.0 degrees) is favored in the solid-state.
C1 [Childs, Bradley C.; Lawler, Keith; Mast, Daniel S.; Forster, Paul M.; Czerwinski, Kenneth R.; Sattelberger, Alfred P.; Poineau, Frederic] UNLV, Dept Chem & Biochem, Las Vegas, NV 89154 USA.
[Lawler, Keith; Mast, Daniel S.; Forster, Paul M.] UNLV, High Pressure Sci & Engn Ctr, Las Vegas, NV 89154 USA.
[Braband, Henrik; Bigler, Laurent; Stalder, Urs; Alberto, Roger] Univ Zurich, Dept Chem, Winterthurerstr 190, CH-8057 Zurich, Switzerland.
[Sattelberger, Alfred P.] Argonne Natl Lab, Lemont, IL 60439 USA.
RP Poineau, F (reprint author), UNLV, Dept Chem & Biochem, Las Vegas, NV 89154 USA.
EM poineauf@unlv.nevada.edu
OI Mast, Daniel/0000-0002-6020-9100
FU Integrated University Program Graduate Fellowship; National Nuclear
Security Administration under the Stewardship Science Academic Alliances
program through DOE [DE-NA0001982]
FX The authors thank Trevor Low and Julie Bertoia (UNLV) for outstanding
health physics support and Joe Gregar (ANL) for fabricating the glass
reactor used for the EI-MS experiment. F.P. acknowledges the Department
of Chemistry and Biochemistry at UNLV for supporting his research
through a startup package. D.M. acknowledges support under an Integrated
University Program Graduate Fellowship. This research was sponsored, in
part, by the National Nuclear Security Administration under the
Stewardship Science Academic Alliances program through DOE Cooperative
Agreement DE-NA0001982.
NR 53
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PU AMER CHEMICAL SOC
PI WASHINGTON
PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA
SN 0020-1669
EI 1520-510X
J9 INORG CHEM
JI Inorg. Chem.
PD OCT 17
PY 2016
VL 55
IS 20
BP 10445
EP 10452
DI 10.1021/acs.inorgchem.6b01683
PG 8
WC Chemistry, Inorganic & Nuclear
SC Chemistry
GA DZ3YL
UT WOS:000385785700059
ER
PT J
AU Sciortino, NF
Ragon, F
Zenere, KA
Southon, PD
Halder, GJ
Chapman, KW
Pineiro-Lopez, L
Real, JA
Kepert, CJ
Neville, SM
AF Sciortino, Natasha F.
Ragon, Florence
Zenere, Katrina A.
Southon, Peter D.
Halder, Gregory J.
Chapman, Karena W.
Pineiro-Lopez, Lucia
Real, Jose A.
Kepert, Cameron J.
Neville, Suzanne M.
TI Exploiting Pressure To Induce a "Guest-Blocked" Spin Transition in a
Framework Material
SO INORGANIC CHEMISTRY
LA English
DT Article
ID CROSSOVER COORDINATION POLYMERS; METAL-ORGANIC FRAMEWORKS;
ROOM-TEMPERATURE; 2D; HYSTERESIS; MODULATION; BEHAVIOR; 2-STEP; STATE;
SYSTEM
AB A new functionalized 1,2,4-triazole ligand, 4-[(E)-2-(5-methyl-2-thienyl)vinyl]-1,2,4-triazole (thiome), was prepared to assess the broad applicability of strategically producing multistep spin transitions in two-dimensional Hofmann-type materials of the type [(FePd)-Pd-II(CN)(4)(R-1,2,4-trz)2]center dot nH(2)O (R-1,2,4-trz = a 4-functionalized 1,2,4-triazole ligand). A variety of structural and magnetic investigations on the resultant framework material [(FePd)-Pd-II-(CN)(4)(thiome)(2)]center dot 2H(2)O (A center dot 2H(2)O) reveal that a high-spin (HS) to low-spin (LS) transition is inhibited in A center dot 2H(2)O due to a combination of guest and ligand steric bulk effects. The water molecules can be reversibly removed with retention of the porous host framework and result in the emergence of an abrupt and hysteretic one-step spin transition due to the removal of guest internal pressure. A spin transition can, furthermore, be induced in A center dot 2H(2)O (00.68 GPa) under hydrostatic pressure, as evidenced by variable-pressure structure and magnetic studies, resulting in a two-step spin transition at ambient temperatures at 0.68 GPa. The presence of a two-step spin crossover (SCO) in A center dot 2H(2)O under hydrostatic pressure compared to a one-step SCO in A at ambient pressure is discussed in terms of the relative ability of each phase to accommodate mixed HS/LS states according to differing lattice flexibilities.
C1 [Sciortino, Natasha F.; Ragon, Florence; Zenere, Katrina A.; Southon, Peter D.; Kepert, Cameron J.; Neville, Suzanne M.] Univ Sydney, Sch Chem, Sydney, NSW 2006, Australia.
[Halder, Gregory J.; Chapman, Karena W.] Argonne Natl Lab, APS, Xray Sci Div, Lemont, IL 60439 USA.
[Pineiro-Lopez, Lucia; Real, Jose A.] Univ Valencia, Inst Ciencia Mol, Valencia 46980, Spain.
RP Neville, SM (reprint author), Univ Sydney, Sch Chem, Sydney, NSW 2006, Australia.
EM suzanne.neville@sydney.edu.au
OI Kepert, Cameron/0000-0002-6105-9706
FU Australian Research Council; U.S. Department of Energy, Office of
Science, Office of Basic Energy Sciences [DE-AC02-06CH11357];
International Synchrotron Access Program; Australian Government; Spanish
Ministerio de Ciencia e Innovacion; FEDER [CTQ2013-46275-P,
MDM-2015-0538]; Generalitat Valenciana [PROMETE02016/147]
FX The Australian Research Council is thanked for providing Discovery
Grants and Research Fellowships to support this work at the University
of Sydney. Access and use of the facilities of the APS was supported by
the U.S. Department of Energy, Office of Science, Office of Basic Energy
Sciences (Contract DE-AC02-06CH11357). Travel to the APS was funded by
the International Synchrotron Access Program managed by the Australian
Synchrotron and funded by the Australian Government. We thank the
Spanish Ministerio de Ciencia e Innovacion and FEDER for funding (Grant
CTQ2013-46275-P and Unidad de Excelencia Maria de Maeztu Grant
MDM-2015-0538) and the Generalitat Valenciana (Grant PROMETE02016/147).
NR 49
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PU AMER CHEMICAL SOC
PI WASHINGTON
PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA
SN 0020-1669
EI 1520-510X
J9 INORG CHEM
JI Inorg. Chem.
PD OCT 17
PY 2016
VL 55
IS 20
BP 10490
EP 10498
DI 10.1021/acs.inorgchem.6b01686
PG 9
WC Chemistry, Inorganic & Nuclear
SC Chemistry
GA DZ3YL
UT WOS:000385785700064
ER
PT J
AU Marjerrison, CA
Thompson, CM
Sala, G
Maharaj, DD
Kermarrec, E
Cai, YP
Hallas, AM
Wilson, MN
Munsie, TJS
Granroth, GE
Flacau, R
Greedan, JE
Gaulin, BD
Luke, GM
AF Marjerrison, Casey A.
Thompson, Corey M.
Sala, Gabrielle
Maharaj, Dalini D.
Kermarrec, Edwin
Cai, Yipeng
Hallas, Alannah M.
Wilson, Murray N.
Munsie, Timothy J. S.
Granroth, Garrett E.
Flacau, Roxana
Greedan, John E.
Gaulin, Bruce D.
Luke, Graeme M.
TI Cubic Re6+ (5d(1)) Double Perovskites, Ba2MgReO6, Ba2ZnReO6, and
Ba2Y2/3ReO6: Magnetism, Heat Capacity, mu SR, and Neutron Scattering
Studies and Comparison with Theory
SO INORGANIC CHEMISTRY
LA English
DT Article
ID RHENIUM
AB Double perovskites (DP) of the general formula Ba2MReO6, where M = Mg, Zn, and Y-2/3, all based on Re6+ (5d(1), t(2g)(1)), were synthesized and studied using magnetization, heat capacity, muon spin relaxation, and neutron-scattering techniques. All are cubic, Fm (3) over barm, at ambient temperature to within the resolution of the X-ray and neutron diffraction data, although the muon data suggest the possibility of a local distortion for M = Mg. The M = Mg DP is a ferromagnet, T-c = 18 K, with a saturation moment similar to 0.3 bohr magnetons at 3 K. There are two anomalies in the heat capacity: a sharp feature at 18 K and a broad maximum centered near 33 K. The total entropy loss below 45 K is 9.68 e.u., which approaches R In 4 (11.52 e.u.) supporting a j = 3/2 ground state. The unit cell constants of Ba2MgReO6 and the isostructural, isoelectronic analogue, Ba2LiOsO6, differ by only 0.1%, yet the latter is an anti-ferromagnet. The M = Zn DP also appears to be a ferromagnet, T-c = 11 K, mu(sat)(Re) = 0.1 mu(B). In this case the heat capacity shows a somewhat broad peak near 10 K and a broader maximum at similar to 33 K, behavior that can be traced to a smaller particle size, similar to 30 nm, for this sample. For both M = Mg and Zn, the low-temperature magnetic heat capacity follows a T-3/2 behavior, consistent with a ferromagnetic spin wave. An attempt to attribute the broad 33 K heat capacity anomalies to a splitting of the j = 3/2 state by a crystal distortion is not supported by inelastic neutron scattering, which shows no transition at the expected energy of similar to 7 meV nor any transition up to 100 meV. However, the results for the two ferromagnets are compared to the theory of Chen, Pereira, and Balents, and the computed heat capacity predicts the two maxima observed experimentally. The M = Y-2/3 DP, with a significantly larger cell constant (3%) than the ferromagnets, shows predominantly anti-ferromagnetic correlations, and the ground state is complex with a spin frozen component T-g = 16 K from both direct current and alternating current susceptibility and mu SR data but with a persistent dynamic component. The low-temperature heat capacity shows a T-1 power law. The unit cell constant of B = Y-2/3 is less than 1% larger than that of the ferromagnetic Os7+ (5d(1)) DP, Ba2NaOsO6.
C1 [Marjerrison, Casey A.; Sala, Gabrielle; Maharaj, Dalini D.; Kermarrec, Edwin; Cai, Yipeng; Hallas, Alannah M.; Wilson, Murray N.; Munsie, Timothy J. S.; Gaulin, Bruce D.; Luke, Graeme M.] McMaster Univ, Dept Phys & Astron, Hamilton, ON L8S 4M1, Canada.
[Thompson, Corey M.; Greedan, John E.] McMaster Univ, Dept Chem & Chem Biol, Hamilton, ON L8S 4M1, Canada.
[Granroth, Garrett E.] Oak Ridge Natl Lab, Quantum Condensed Matter Div, Oak Ridge, TN 37831 USA.
[Flacau, Roxana] Canadian Nucl Labs, Canadian Neutron Beam Ctr, Chalk River, ON K0J 1J0, Canada.
[Greedan, John E.; Gaulin, Bruce D.; Luke, Graeme M.] Brockhouse Inst Mat Res, Hamilton, ON L8S 4M1, Canada.
[Gaulin, Bruce D.; Luke, Graeme M.] Canadian Inst Adv Res, 180 Dundas St W, Toronto, ON MSG 1Z8, Canada.
RP Greedan, JE (reprint author), McMaster Univ, Dept Chem & Chem Biol, Hamilton, ON L8S 4M1, Canada.; Greedan, JE (reprint author), Brockhouse Inst Mat Res, Hamilton, ON L8S 4M1, Canada.
EM greedan@mcmaster.ca
RI Granroth, Garrett/G-3576-2012; Luke, Graeme/A-9094-2010
OI Granroth, Garrett/0000-0002-7583-8778;
FU Natural Sciences and Engineering Research Council of Canada via the
Discovery Grant Program; Scientific User Facilities Division, Office of
Basic Energy Sciences, U.S. Department of Energy
FX J.E.G., G.M.L., and B.D.G. thank the Natural Sciences and Engineering
Research Council of Canada for support via the Discovery Grant Program.
P. Dube assisted with collection of magnetization and heat capacity
data. We thank the TRIUMF CMMS staff for invaluable assistance with the
mu SR experiments. Research at Oak Ridge National Laboratory's
Spallation Neutron Source was sponsored by the Scientific User
Facilities Division, Office of Basic Energy Sciences, U.S. Department of
Energy.
NR 34
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PU AMER CHEMICAL SOC
PI WASHINGTON
PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA
SN 0020-1669
EI 1520-510X
J9 INORG CHEM
JI Inorg. Chem.
PD OCT 17
PY 2016
VL 55
IS 20
BP 10701
EP 10713
DI 10.1021/acs.inorgchem.6b01933
PG 13
WC Chemistry, Inorganic & Nuclear
SC Chemistry
GA DZ3YL
UT WOS:000385785700084
ER
PT J
AU Santamaria-Perez, D
McGuire, C
Makhluf, A
Kavner, A
Chulia-Jordan, R
Pellicer-Porres, J
Martinez-Garcia, D
Doran, A
Kunz, M
Rodriguez-Hernandez, P
Munoz, A
AF Santamaria-Perez, David
McGuire, Chris
Makhluf, Adam
Kavner, Abby
Chulia-Jordan, Raquel
Pellicer-Porres, Julio
Martinez-Garcia, Domingo
Doran, Andrew
Kunz, Martin
Rodriguez-Hernandez, Placida
Munoz, Alfonso
TI Exploring the Chemical Reactivity between Carbon Dioxide and Three
Transition Metals (Au, Pt, and Re) at High-Pressure, High Temperature
Conditions
SO INORGANIC CHEMISTRY
LA English
DT Article
ID X-RAY-DIFFRACTION; CO2; REDUCTION; STABILITY; DYNAMICS; SURFACES;
RHENIUM; OXIDE; NI
AB The role of carbon dioxide, CO2, as oxidizing agent at high pressures and temperatures is evaluated by studying its chemical reactivity with three transition metals: Au, Pt, and Re. We report systematic X-ray diffraction measurements up to 48 GPa and 2400 K using synchrotron radiation and laser-heating diamond-anvil cells. No evidence of reaction was found in Au and Pt samples in this pressure temperature range. In the Re + CO2 system, however, a strongly driven redox reaction occurs at P > 8 GPa and T > 1500 K, and orthorhombic beta-ReO2 is formed. This rhenium oxide phase is stable at least up to 48 GPa and 2400 K and was recovered at ambient conditions. Raman spectroscopy data confirm graphite as a reaction product. Ab-initio total-energy structural and compressibility data of the beta-ReO2 phase shows an excellent agreement with experiments, altogether accurately confirming CO, reduction P T conditions in the presence of rhenium metal' and the beta-ReO2 equation of state.
C1 [Santamaria-Perez, David; McGuire, Chris; Makhluf, Adam; Kavner, Abby] Univ Calif Los Angeles, Earth Planetary & Space Sci Dept, Los Angeles, CA 90095 USA.
[Santamaria-Perez, David; Chulia-Jordan, Raquel; Pellicer-Porres, Julio; Martinez-Garcia, Domingo] Univ Valencia, Dept Fis Aplicada ICMUV, E-46100 Valencia, Spain.
[Doran, Andrew; Kunz, Martin] Lawrence Berkeley Natl Lab, Adv Light Source, Berkeley, CA 94720 USA.
[Rodriguez-Hernandez, Placida; Munoz, Alfonso] Univ La Laguna, Inst Univ Mat & Nanotecnol, Dept Fis, San Cristobal la Laguna 38206, Tenerife, Spain.
RP Santamaria-Perez, D (reprint author), Univ Calif Los Angeles, Earth Planetary & Space Sci Dept, Los Angeles, CA 90095 USA.; Santamaria-Perez, D (reprint author), Univ Valencia, Dept Fis Aplicada ICMUV, E-46100 Valencia, Spain.
EM David.Santamaria@uv.es
RI Munoz, Alfonso/K-7823-2013; Pellicer Porres, Julio/K-4234-2015;
Santamaria-Perez, David/A-2486-2012; Rodriguez-Hernandez,
Placida/E-8218-2017;
OI Munoz, Alfonso/0000-0003-3347-6518; Pellicer Porres,
Julio/0000-0002-4288-900X; Santamaria-Perez, David/0000-0002-1119-5056;
Rodriguez-Hernandez, Placida/0000-0002-4148-6516; Doran,
Andrew/0000-0001-5158-4569
FU Marie Curie Action [PIOF-GA-2013-622439]; Spanish Consolider Ingenio
Program [CSD2007-00045]; Spanish government MEC
[MAT2013-46649-C4-1/3-P]; Deep Carbon Observatory; National Science
Foundation - Earth Sciences [EAR-1128799]; Department of - Energy -
GeoSciences [DE-FG02-94ER14466]; DOE Office of Science
[DE-AC02-06CH11357]; COMPRES under NSF [EAR 11-57758]; Office of
Science, Office of Basic Energy Sciences, of the U.S. Department of
Energy [DE-AC02-05CH11231]; COMPRES, the Consortium for Materials
Properties Research in Earth Sciences under NSF [EAR 10-43050]
FX This work was supported by the Marie Curie Action PIOF-GA-2013-622439.
Financial support from the Spanish Consolider Ingenio 2010 Program
(Project No. CSD2007-00045), the Spanish government MEC under Grant No.
MAT2013-46649-C4-1/3-P, and the Deep Carbon Observatory is also
acknowledged. Supercomputer time has been provided by the Red Espanola
de Supercomputacion (RES) and the MALTA cluster. Portions of this work
were performed at GeoSoilEnviroCARS (Sector 13), Advanced Photon Source
(APS), and Argonne National Laboratory. GeoSoilEnviroCARS is supported
by the National Science Foundation - Earth Sciences (EAR-1128799) and
Department of - Energy - GeoSciences (DE-FG02-94ER14466). This research
used resources of the Advanced Photon Source, a U.S. Department of
Energy (DOE) Office of Science User Facility operated for the DOE Office
of Science by Argonne National Laboratory under Contract No.
DE-AC02-06CH11357. Use of the COMPRES-GSECARS gas loading system was
supported by COMPRES under NSF Cooperative Agreement EAR 11-57758. The
Advanced Light Source is supported by the Director, Office of Science,
Office of Basic Energy Sciences, of the U.S. Department of Energy under
Contract No. DE-AC02-05CH11231. Use of the beamline 12.2.2 at the ALS is
supported by COMPRES, the Consortium for Materials Properties Research
in Earth Sciences under NSF Cooperative Agreement EAR 10-43050.
NR 39
TC 1
Z9 1
U1 8
U2 8
PU AMER CHEMICAL SOC
PI WASHINGTON
PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA
SN 0020-1669
EI 1520-510X
J9 INORG CHEM
JI Inorg. Chem.
PD OCT 17
PY 2016
VL 55
IS 20
BP 10793
EP 10799
DI 10.1021/acs.inorgchem.6b01858
PG 7
WC Chemistry, Inorganic & Nuclear
SC Chemistry
GA DZ3YL
UT WOS:000385785700092
ER
PT J
AU Lashley, MA
Ivanov, AS
Bryantsev, VS
Dai, S
Hancock, RD
AF Lashley, Mark A.
Ivanov, Alexander S.
Bryantsev, Vyacheslav S.
Dai, Sheng
Hancock, Robert D.
TI Highly Preorganized Ligand 1,10-Phenanthroline-2,9-dicarboxylic Acid for
the Selective Recovery of Uranium from Seawater in the Presence of
Competing Vanadium Species
SO INORGANIC CHEMISTRY
LA English
DT Article
ID METAL-IONS; AQUEOUS-SOLUTION; URANYL COMPLEXES; STABILITY-CONSTANTS;
INTERNAL-ROTATION; BINDING STRENGTH; ELECTRON-DENSITY; HIGHER CHARGE;
EXTRACTION; AMIDOXIME
AB Studies of the complexation of new promising ligands with uranyl (UO22+) and other seawater cations can aid the development of more efficient, selective, and robust sorbents for the recovery of uranium from seawater. In this work, we propose that the ligand design principles based on structural preorganization can be successfully applied to obtain a dramatic enhancement in UO22+ ion binding affinity and selectivity. This concept is exemplified through the investigation of the complexes of UO22++, VO2+, and VO2+ with the highly preorganized ligand 1,10-phenanthroline-2,9-dicarboxylic acid (PDA) using a combination of fluorescence and absorbance techniques, along with density functional theory (DFT) calculations. The measured stability constant value, log K-1, of 16.5 for the UO22+/PDA complex is very high compared to uranyl complexes with other dicarboxylic ligands. Moreover, PDA exhibits strong selectivity for uranyl over vanadium ions, since the determined stability constant values of the PDA complexes of the vanadium ions are quite low (V(IV) log K-1 = 7.4, V(V) = 7.3). The structures of the corresponding UO22+, VO2+, and VO2+ complexes with PDA were identified by systematic DFT calculations and helped to interpret the stronger binding affinity for uranium over the vanadium ions. Because of its high chemical stability, selectivity, and structural preorganization for UO22+ complexation, PDA is a very promising candidate that can be potentially used in the development of novel adsorbent materials for the selective extraction of uranium from seawater.
C1 [Ivanov, Alexander S.; Bryantsev, Vyacheslav S.; Dai, Sheng] Univ N Carolina, Dept Chem & Biochem, Wilmington, NC 28403 USA.
[Lashley, Mark A.; Hancock, Robert D.] Oak Ridge Natl Lab, Div Chem Sci, 1 Bethel Valley Rd, Oak Ridge, TN 37831 USA.
RP Bryantsev, VS (reprint author), Univ N Carolina, Dept Chem & Biochem, Wilmington, NC 28403 USA.; Hancock, RD (reprint author), Oak Ridge Natl Lab, Div Chem Sci, 1 Bethel Valley Rd, Oak Ridge, TN 37831 USA.
EM bryantsevv@ornl.gov; hancockr@uncw.edu
FU U.S. Department of Energy, Office of Nuclear Energy [DE-AC05-00OR22725];
Oak Ridge National Laboratory
FX This work was sponsored by the U.S. Department of Energy, Office of
Nuclear Energy, under Contract DE-AC05-00OR22725 with Oak Ridge National
Laboratory, managed by UT-Battelle, LLC.
NR 74
TC 0
Z9 0
U1 29
U2 29
PU AMER CHEMICAL SOC
PI WASHINGTON
PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA
SN 0020-1669
EI 1520-510X
J9 INORG CHEM
JI Inorg. Chem.
PD OCT 17
PY 2016
VL 55
IS 20
BP 10818
EP 10829
DI 10.1021/acs.inorgchem.6b02234
PG 12
WC Chemistry, Inorganic & Nuclear
SC Chemistry
GA DZ3YL
UT WOS:000385785700095
PM 27689540
ER
PT J
AU Xu, LY
Chen, DG
Itoh, T
Reno, JL
Williams, BS
AF Xu, Luyao
Chen, Daguan
Itoh, Tatsuo
Reno, John L.
Williams, Benjamin S.
TI Focusing metasurface quantum-cascade laser with a near
diffraction-limited beam
SO OPTICS EXPRESS
LA English
DT Article
ID EMITTING SEMICONDUCTOR-LASERS; MESH COUPLERS; TERAHERTZ; REFLECTARRAY;
METAMATERIALS; ARRAYS; MODEL; POWER
AB A terahertz vertical-external-cavity surface-emitting-laser (VECSEL) is demonstrated using an active focusing reflectarray metasurface based on quantum-cascade gain material. The focusing effect enables a hemispherical cavity with flat optics, which exhibits higher geometric stability than a plano-plano cavity and a directive and circular near-diffraction limited Gaussian beam with M-2 beam parameter as low as 1.3 and brightness of 1.86 x 10(6) W sr(-1)m(-2). This work initiates the potential of leveraging inhomogeneous metasurface and reflectarray designs to achieve high-power and high-brightness terahertz quantum-cascade VECSELs. (C) 2016 Optical Society of America
C1 [Xu, Luyao; Chen, Daguan; Itoh, Tatsuo; Williams, Benjamin S.] Univ Calif Los Angeles, Dept Elect Engn, Los Angeles, CA 90095 USA.
[Xu, Luyao; Williams, Benjamin S.] Univ Calif Los Angeles, Calif NanoSyst Inst, Los Angeles, CA 90095 USA.
[Reno, John L.] Ctr Integrated Nanotechnol, Sandia Natl Labs, MS 1303, Albuquerque, NM 87185 USA.
RP Williams, BS (reprint author), Univ Calif Los Angeles, Dept Elect Engn, Los Angeles, CA 90095 USA.; Williams, BS (reprint author), Univ Calif Los Angeles, Calif NanoSyst Inst, Los Angeles, CA 90095 USA.
EM bswilliams@ucla.edu
RI Williams, Benjamin/B-4494-2013
OI Williams, Benjamin/0000-0002-6241-8336
FU National Science Foundation (NSF) [1150071, 1407711]; National
Aeronautics and Space Administration (NASA) [NNX16AC73G]
FX National Science Foundation (NSF) (1150071, 1407711), National
Aeronautics and Space Administration (NASA) (NNX16AC73G).
NR 33
TC 0
Z9 0
U1 13
U2 13
PU OPTICAL SOC AMER
PI WASHINGTON
PA 2010 MASSACHUSETTS AVE NW, WASHINGTON, DC 20036 USA
SN 1094-4087
J9 OPT EXPRESS
JI Opt. Express
PD OCT 17
PY 2016
VL 24
IS 21
BP 24117
EP 24128
DI 10.1364/OE.24.024117
PG 12
WC Optics
SC Optics
GA EC8NR
UT WOS:000388399100043
PM 27828242
ER
PT J
AU Huang, L
Xue, JP
Gao, B
McPherson, C
Beverage, J
Idir, M
AF Huang, Lei
Xue, Junpeng
Gao, Bo
McPherson, Chris
Beverage, Jacob
Idir, Mourad
TI Modal phase measuring deflectometry
SO OPTICS EXPRESS
LA English
DT Article
ID WAVE-FRONT RECONSTRUCTION; 3D SHAPE MEASUREMENT; ZERNIKE POLYNOMIALS;
FRINGE REFLECTOMETRY; REFLECTION; CALIBRATION; SURFACES; GRADIENT;
MIRROR
AB In this work, a model based method is applied to phase measuring deflectometry, named modal phase measuring deflectometry. The height and slopes of the surface under test are represented by mathematical models and updated by optimizing the model coefficients to minimize the discrepancy between the reprojection in ray tracing and the actual measurement. The pose of the screen relative to the camera is pre-calibrated and further optimized together with the shape coefficients of the surface under test. Simulations and experiments are conducted to demonstrate the feasibility of the proposed approach. (C) 2016 Optical Society of America
C1 [Huang, Lei; Xue, Junpeng; Gao, Bo; Idir, Mourad] Brookhaven Natl Lab, NSLS II, 50 Rutherford Dr, Upton, NY 11973 USA.
[Xue, Junpeng] Sichuan Univ, Sch Aeronaut & Astronaut, Chengdu 610065, Peoples R China.
[Gao, Bo] Chinese Acad Sci, Shanghai Inst Appl Phys, Shanghai 201800, Peoples R China.
[Gao, Bo] Univ Chinese Acad Sci, Beijing 100049, Peoples R China.
[McPherson, Chris; Beverage, Jacob] Arizona Opt Syst, Tucson, AZ 85747 USA.
RP Huang, L (reprint author), Brookhaven Natl Lab, NSLS II, 50 Rutherford Dr, Upton, NY 11973 USA.
EM huanglei0114@gmail.com
FU US Department of Energy, Office of Science, Office of Basic Energy
Sciences [DE-AC-02-98CH10886]
FX US Department of Energy, Office of Science, Office of Basic Energy
Sciences (contract No. DE-AC-02-98CH10886).
NR 33
TC 2
Z9 2
U1 6
U2 6
PU OPTICAL SOC AMER
PI WASHINGTON
PA 2010 MASSACHUSETTS AVE NW, WASHINGTON, DC 20036 USA
SN 1094-4087
J9 OPT EXPRESS
JI Opt. Express
PD OCT 17
PY 2016
VL 24
IS 21
BP 24649
EP 24664
DI 10.1364/OE.24.024649
PG 16
WC Optics
SC Optics
GA EC8NR
UT WOS:000388399100090
PM 27828190
ER
PT J
AU Tripathi, A
Mcnulty, I
Munson, T
Wild, SM
AF Tripathi, Ashish
Mcnulty, Ian
Munson, Todd
Wild, Stefan M.
TI Single-view phase retrieval of an extended sample by exploiting edge
detection and sparsity
SO OPTICS EXPRESS
LA English
DT Article
ID RAY-DIFFRACTION MICROSCOPY; ALGORITHMS; RECONSTRUCTION; MINIMIZATION
AB We propose a new approach to robustly retrieve the exit wave of an extended sample from its coherent diffraction pattern by exploiting sparsity of the sample's edges. This approach enables imaging of an extended sample with a single view, without ptychography. We introduce nonlinear optimization methods that promote sparsity, and we derive update rules to robustly recover the sample's exit wave. We test these methods on simulated samples by varying the sparsity of the edge-detected representation of the exit wave. Our tests illustrate the strengths and limitations of the proposed method in imaging extended samples. (C) 2016 Optical Society of America
C1 [Tripathi, Ashish; Munson, Todd; Wild, Stefan M.] Argonne Natl Lab, Math & Comp Sci Div, Lemont, IL 60439 USA.
[Mcnulty, Ian] Argonne Natl Lab, Ctr Nanoscale Mat, Lemont, IL 60439 USA.
RP Tripathi, A (reprint author), Argonne Natl Lab, Math & Comp Sci Div, Lemont, IL 60439 USA.
EM atripathi@mcs.anl.gov
FU U.S. Department of Energy, Office of Science, Offices of Advanced
Scientific Computing Research and Basic Energy Sciences
[DE-AC02-06CH11357]
FX U.S. Department of Energy, Office of Science, Offices of Advanced
Scientific Computing Research and Basic Energy Sciences under Contract
No. DE-AC02-06CH11357.
NR 39
TC 0
Z9 0
U1 2
U2 2
PU OPTICAL SOC AMER
PI WASHINGTON
PA 2010 MASSACHUSETTS AVE NW, WASHINGTON, DC 20036 USA
SN 1094-4087
J9 OPT EXPRESS
JI Opt. Express
PD OCT 17
PY 2016
VL 24
IS 21
BP 24719
EP 24738
DI 10.1364/OE.24.024719
PG 20
WC Optics
SC Optics
GA EC8NR
UT WOS:000388399100093
PM 27828193
ER
PT J
AU Ishikawa, R
Pennycook, SJ
Lupini, AR
Findlay, SD
Shibata, N
Ikuhara, Y
AF Ishikawa, Ryo
Pennycook, Stephen J.
Lupini, Andrew R.
Findlay, Scott D.
Shibata, Naoya
Ikuhara, Yuichi
TI Single atom visibility in STEM optical depth sectioning
SO APPLIED PHYSICS LETTERS
LA English
DT Article
ID TRANSMISSION ELECTRON-MICROSCOPY; ABERRATION-CORRECTED STEM; FIELD;
SPECTROSCOPY; SCATTERING; RESOLUTION; DOPANT; IMAGE; SI
AB The continuing development of aberration correctors for the scanning transmission electron microscope (STEM) offers the possibility of locating single atoms in crystals in 3D via optical depth sectioning. The main factors that determine the feasibility of such an approach are visibility and dose requirements. Here, we show how Poisson's statistics can be quantitatively incorporated into STEM image simulations and demonstrate that the 3D location of single cerium atoms in wurtzite-type aluminum nitride is indeed feasible under large-angle illumination conditions with a relatively low dose. We also show that chromatic aberration does not presently represent a limitation provided a cold field emission source is used. These results suggest efforts into improved aberration corrector designs for larger illumination angles that offer significant potential for 3D structure determination of materials. Published by AIP Publishing.
C1 [Ishikawa, Ryo; Shibata, Naoya; Ikuhara, Yuichi] Univ Tokyo, Inst Engn Innovat, Bunkyo Ku, Tokyo 1138656, Japan.
[Pennycook, Stephen J.] Natl Univ Singapore, Dept Mat Sci & Engn, Singapore 177576, Singapore.
[Lupini, Andrew R.] Oak Ridge Natl Lab, Mat Sci & Technol Div, Oak Ridge, TN 37831 USA.
[Findlay, Scott D.] Monash Univ, Sch Phys & Astron, Clayton, Vic 3800, Australia.
[Ikuhara, Yuichi] Japan Fine Ceram Ctr, Nanostruct Res Lab, Nagoya, Aichi 4568587, Japan.
RP Ishikawa, R (reprint author), Univ Tokyo, Inst Engn Innovat, Bunkyo Ku, Tokyo 1138656, Japan.
EM ishikawa@sigma.t.u-tokyo.ac.jp
RI Shibata, Naoya/E-5327-2013; Ikuhara, Yuichi/F-3066-2010;
OI Findlay, Scott/0000-0003-4862-4827; Ishikawa, Ryo/0000-0001-5801-0971
FU Research and Development Initiative for Scientific Innovation of New
Generation Batteries (RISING II) project of the New Energy and
Industrial Technology Development Organization (NEDO), Japan; Office of
Science of the U.S. Department of Energy [DE-AC02-05CH11231]; Office of
Basic Energy Sciences, Materials Sciences and Engineering Division, U.S.
Department of Energy; Australian Research Council [DP110102228]
FX A part of this work was supported by the Research and Development
Initiative for Scientific Innovation of New Generation Batteries (RISING
II) project of the New Energy and Industrial Technology Development
Organization (NEDO), Japan. R.I. used resources of the National Energy
Research Scientific Computing Center, which was supported by the Office
of Science of the U.S. Department of Energy under Contract No.
DE-AC02-05CH11231, A.R.L. was supported by the Office of Basic Energy
Sciences, Materials Sciences and Engineering Division, U.S. Department
of Energy. This research was supported under the Australian Research
Council's Discovery Projects funding scheme (Project No. DP110102228).
NR 30
TC 0
Z9 0
U1 14
U2 14
PU AMER INST PHYSICS
PI MELVILLE
PA 1305 WALT WHITMAN RD, STE 300, MELVILLE, NY 11747-4501 USA
SN 0003-6951
EI 1077-3118
J9 APPL PHYS LETT
JI Appl. Phys. Lett.
PD OCT 17
PY 2016
VL 109
IS 16
AR 163102
DI 10.1063/1.4965709
PG 5
WC Physics, Applied
SC Physics
GA EA9AT
UT WOS:000386933200032
ER
PT J
AU Kovarik, L
Stevens, A
Liyu, A
Browning, ND
AF Kovarik, L.
Stevens, A.
Liyu, A.
Browning, N. D.
TI Implementing an accurate and rapid sparse sampling approach for low-dose
atomic resolution STEM imaging
SO APPLIED PHYSICS LETTERS
LA English
DT Article
ID TRANSMISSION ELECTRON-MICROSCOPY; RADIATION-DAMAGE; TOMOGRAPHY;
RECONSTRUCTION; INFORMATION; IMAGES; TEM
AB While aberration correction for scanning transmission electron microscopes (STEMs) dramatically increased the spatial resolution obtainable in the images of materials that are stable under the electron beam, the practical resolution of many STEM images is now limited by the sample stability rather than the microscope. To extract physical information from the images of beam sensitive materials, it is becoming clear that there is a critical dose/dose-rate below which the images can be interpreted as representative of the pristine material, while above it the observation is dominated by beam effects. Here, we describe an experimental approach for sparse sampling in the STEM and in-painting image reconstruction in order to reduce the electron dose/dose-rate to the sample during imaging. By characterizing the induction limited rise-time and hysteresis in the scan coils, we show that a sparse line-hopping approach to scan randomization can be implemented that optimizes both the speed of the scan and the amount of the sample that needs to be illuminated by the beam. The dose and acquisition time for the sparse sampling is shown to be effectively decreased by at least a factor of 5 x relative to conventional acquisition, permitting imaging of beam sensitive materials to be obtained without changing the microscope operating parameters. The use of sparse line-hopping scan to acquire STEM images is demonstrated with atomic resolution aberration corrected the Z-contrast images of CaCO3, a material that is traditionally difficult to image by TEM/STEM because of dosage issues. Published by AIP Publishing.
C1 [Kovarik, L.; Liyu, A.] Pacific Northwest Natl Lab, Environm Mol Sci Lab, Richland, WA 99352 USA.
[Stevens, A.] Pacific Northwest Natl Lab, Natl Secur Directorate, Richland, WA 99352 USA.
[Stevens, A.] Duke Univ, Elect & Comp Engn, Durham, NC 27705 USA.
[Browning, N. D.] Pacific Northwest Natl Lab, Phys & Computat Sci Directorate, Richland, WA 99352 USA.
[Browning, N. D.] Univ Washington, Mat Sci & Engn, Seattle, WA 98195 USA.
RP Kovarik, L (reprint author), Pacific Northwest Natl Lab, Environm Mol Sci Lab, Richland, WA 99352 USA.
EM libor.kovarik@pnl.gov
OI Stevens, Andrew/0000-0002-8474-8483
FU Chemical Imaging Initiative, a Laboratory Directed Research and
Development Program at Pacific Northwest National Laboratory (PNNL);
U.S. Department of Energy (DOE) [DE-AC05-76RL01830]; Department of
Energy's Office of Biological and Environmental Research
FX The development of Compressive sensing for EM applications was supported
by the Chemical Imaging Initiative, a Laboratory Directed Research and
Development Program at Pacific Northwest National Laboratory (PNNL).
PNNL is a multi-program national laboratory operated by Battelle for the
U.S. Department of Energy (DOE) under Contract No. DE-AC05-76RL01830. A
portion of the research was performed using the Environmental Molecular
Sciences Laboratory (EMSL), a national scientific user facility
sponsored by the Department of Energy's Office of Biological and
Environmental Research and located at PNNL. We would like to acknowledge
Dr. Tamas Varga and Dr. Sebastien Kerisit for their kind help in
providing samples for this study.
NR 32
TC 1
Z9 1
U1 11
U2 11
PU AMER INST PHYSICS
PI MELVILLE
PA 1305 WALT WHITMAN RD, STE 300, MELVILLE, NY 11747-4501 USA
SN 0003-6951
EI 1077-3118
J9 APPL PHYS LETT
JI Appl. Phys. Lett.
PD OCT 17
PY 2016
VL 109
IS 16
AR 164102
DI 10.1063/1.4965720
PG 5
WC Physics, Applied
SC Physics
GA EA9AT
UT WOS:000386933200048
ER
PT J
AU Majdi, S
Gabrysch, M
Kovi, KK
Suntornwipat, N
Friel, I
Isberg, J
AF Majdi, S.
Gabrysch, M.
Kovi, K. K.
Suntornwipat, N.
Friel, I.
Isberg, J.
TI Low temperature conduction-band transport in diamond
SO APPLIED PHYSICS LETTERS
LA English
DT Article
ID SINGLE-CRYSTAL DIAMOND; HOLE-DRIFT VELOCITY; CVD-DIAMOND;
CYCLOTRON-RESONANCE; DEPOSITED DIAMOND; CHARGE-TRANSPORT; EFFECTIVE
MASSES; NATURAL DIAMOND; MOBILITY; SCATTERING
AB By performing Time-of-Flight measurements on high-purity single-crystalline chemical vapor deposited diamond, we are able to extract the electron drift velocity of valley-polarized electrons in the low-injection regime. The aim of this study is to improve the understanding of the mechanisms involved in the conduction-band transport of valley-polarized electrons. The measurements were carried out within the temperature range of 10-80 K, and the experimental results are systematically compared with Monte Carlo charge transport simulations. We observe a rapid enhancement of the electron mobility with decreasing temperature, which reveals that inelastic effects in electron-phonon scattering become important below similar to 40 K. In addition, we obtain the momentum relaxation rate for electrons with different valley polarizations. Published by AIP Publishing.
C1 [Majdi, S.; Gabrysch, M.; Kovi, K. K.; Suntornwipat, N.; Isberg, J.] Uppsala Univ, Dept Engn Sci, Div Elect, Box 534, S-75121 Uppsala, Sweden.
[Kovi, K. K.] Argonne Natl Lab, Ctr Nanoscale Mat, Argonne, IL 60439 USA.
[Friel, I.] Element Six Innovat, Fermi Ave, Didcot OX11 0QR, Oxon, England.
RP Majdi, S (reprint author), Uppsala Univ, Dept Engn Sci, Div Elect, Box 534, S-75121 Uppsala, Sweden.
EM Saman.Majdi@angstrom.uu.se
OI Kovi, Kiran Kumar/0000-0003-0669-9476; Isberg, Jan/0000-0003-2197-5352
FU Swedish Research Council (VR) [621-2014-6026]; AForsk Foundation
[15-288]; Carl Tryggers Foundation [14:151, 15:225]; Swedish National
Infrastructure for Computing through Uppsala Multidisciplinary Center
for Advanced Computational Science (UPPMAX) [SNIC2014-3-65]
FX The authors would like to thank the Swedish Research Council (VR, Grant
No. 621-2014-6026), the AForsk Foundation (Grant No. 15-288) and the
Carl Tryggers Foundation (Grants Nos. 14:151 and 15:225) for financial
support. The Monte Carlo simulations were performed on resources
provided by the Swedish National Infrastructure for Computing through
Uppsala Multidisciplinary Center for Advanced Computational Science
(UPPMAX) under Project SNIC2014-3-65.
NR 37
TC 0
Z9 0
U1 6
U2 6
PU AMER INST PHYSICS
PI MELVILLE
PA 1305 WALT WHITMAN RD, STE 300, MELVILLE, NY 11747-4501 USA
SN 0003-6951
EI 1077-3118
J9 APPL PHYS LETT
JI Appl. Phys. Lett.
PD OCT 17
PY 2016
VL 109
IS 16
AR 162106
DI 10.1063/1.4964720
PG 5
WC Physics, Applied
SC Physics
GA EA9AT
UT WOS:000386933200020
ER
PT J
AU Rodriguez, G
Smilowitz, L
Henson, BF
AF Rodriguez, G.
Smilowitz, L.
Henson, B. F.
TI Embedded fiber Bragg grating pressure measurement during thermal
ignition of a high explosive
SO APPLIED PHYSICS LETTERS
LA English
DT Article
ID COOK-OFF; HMX; VIOLENCE; STRAIN
AB A high-speed fiber Bragg grating based pressure-only measurement is reported for the high explosive PBXN-9 under thermal initiation conditions. During exothermic thermal runaway, an explosion rise time of 500 mu s reaching a peak pressure of 660 MPa is measured. The approach offers a direct measure pressure diagnostic useful for quantifying reaction violence for high explosive chemistry. Published by AIP Publishing.
C1 [Rodriguez, G.] Los Alamos Natl Lab, MPA CINT, Mail Stop K771, Los Alamos, NM 87545 USA.
[Smilowitz, L.; Henson, B. F.] Los Alamos Natl Lab, C PCS, Mail Stop J567, Los Alamos, NM 87545 USA.
RP Rodriguez, G (reprint author), Los Alamos Natl Lab, MPA CINT, Mail Stop K771, Los Alamos, NM 87545 USA.
EM rodrigeo@lanl.gov
RI Rodriguez, George/G-7571-2012
OI Rodriguez, George/0000-0002-6044-9462
FU DOE/NNSA Science Campaign 2; Laboratory Directed Research and
Development program; DOD/DOE Joint Munitions Program at Los Alamos
National Laboratory of the U.S. Department of Energy for Los Alamos
National Security, LLC [DE-AC52-06NA25396]
FX This work was supported by the DOE/NNSA Science Campaign 2, the
Laboratory Directed Research and Development program, and the DOD/DOE
Joint Munitions Program at Los Alamos National Laboratory under the
auspices of the U.S. Department of Energy for Los Alamos National
Security, LLC. Contract. No. DE-AC52-06NA25396.
NR 20
TC 1
Z9 1
U1 2
U2 2
PU AMER INST PHYSICS
PI MELVILLE
PA 1305 WALT WHITMAN RD, STE 300, MELVILLE, NY 11747-4501 USA
SN 0003-6951
EI 1077-3118
J9 APPL PHYS LETT
JI Appl. Phys. Lett.
PD OCT 17
PY 2016
VL 109
IS 16
AR 164101
DI 10.1063/1.4965842
PG 5
WC Physics, Applied
SC Physics
GA EA9AT
UT WOS:000386933200047
ER
PT J
AU Stone, KH
Christensen, ST
Harvey, SP
Teeter, G
Repins, IL
Toney, MF
AF Stone, Kevin H.
Christensen, Steven T.
Harvey, Steven P.
Teeter, Glenn
Repins, Ingrid L.
Toney, Michael F.
TI Quantifying point defects in Cu2ZnSn(S,Se)(4) thin films using resonant
x-ray diffraction
SO APPLIED PHYSICS LETTERS
LA English
DT Article
ID KESTERITE CU2ZNSNS4; SOLAR-CELLS; EFFICIENCY; CHALCOGENIDES
AB Cu2ZnSn(S,Se)(4) is an interesting, earth abundant photovoltaic material, but has suffered from low open circuit voltage. To better understand the film structure, we have measured resonant x-ray diffraction across the Cu and Zn K-edges for the device quality thin films of Cu2ZnSnS4 (8.6% efficiency) and Cu2ZnSn(S,Se)(4) (3.5% efficiency). This approach allows for the confirmation of the underlying kesterite structure and quantification of the concentration of point defects and vacancies on the Cu, Zn, and Sn sublattices. Rietveld refinement of powder diffraction data collected at multiple energies is used to determine that there exists a high level of Cu-Zn and Zn-Cu defects on the 2c and 2d Wyckoff positions. We observe a significantly lower concentration of Zn-Sn defects and Cu or Zn vacancies. Published by AIP Publishing.
C1 [Stone, Kevin H.; Toney, Michael F.] SLAC Natl Accelerator Lab, Stanford Synchrotron Radiat Lightsource, Menlo Pk, CA 94025 USA.
[Christensen, Steven T.; Harvey, Steven P.; Teeter, Glenn; Repins, Ingrid L.] Natl Renewable Energy Lab, Golden, CO 80401 USA.
RP Stone, KH (reprint author), SLAC Natl Accelerator Lab, Stanford Synchrotron Radiat Lightsource, Menlo Pk, CA 94025 USA.
OI Teeter, Glenn/0000-0001-8202-8477
FU U.S. Department of Energy, Office of Science, Office of Basic Energy
Sciences as part of the DOE Energy Frontier Research Center "Center for
Inverse Design" [DE-AC36-08GO28308]; U.S. Department of Energy, Office
of Basic Energy Sciences [DE-AC02-76SF00515]
FX The authors would like to thank Charles Troxel, Jr. for his assistance
with SSRL beamline 2-1 where these measurements were performed. This
work was supported by the U.S. Department of Energy, Office of Science,
Office of Basic Energy Sciences under Contract No. DE-AC36-08GO28308 as
part of the DOE Energy Frontier Research Center "Center for Inverse
Design." Use of the Stanford Synchrotron Radiation Lightsource, SLAC
National Accelerator Laboratory, was supported by the U.S. Department of
Energy, Office of Basic Energy Sciences under Contract No.
DE-AC02-76SF00515.
NR 23
TC 0
Z9 0
U1 8
U2 8
PU AMER INST PHYSICS
PI MELVILLE
PA 1305 WALT WHITMAN RD, STE 300, MELVILLE, NY 11747-4501 USA
SN 0003-6951
EI 1077-3118
J9 APPL PHYS LETT
JI Appl. Phys. Lett.
PD OCT 17
PY 2016
VL 109
IS 16
AR 161901
DI 10.1063/1.4964738
PG 4
WC Physics, Applied
SC Physics
GA EA9AT
UT WOS:000386933200010
ER
PT J
AU Thompson, J
Nichols, J
Lee, S
Ryee, S
Gruenewald, JH
Connell, JG
Souri, M
Johnson, JM
Hwang, J
Han, MJ
Lee, HN
Kim, DW
Seo, SSA
AF Thompson, J.
Nichols, J.
Lee, S.
Ryee, S.
Gruenewald, J. H.
Connell, J. G.
Souri, M.
Johnson, J. M.
Hwang, J.
Han, M. J.
Lee, H. N.
Kim, D. -W.
Seo, S. S. A.
TI Enhanced metallic properties of SrRuO3 thin films via kinetically
controlled pulsed laser epitaxy
SO APPLIED PHYSICS LETTERS
LA English
DT Article
ID ELECTRONIC-STRUCTURE; MEMORY; INTERFACES; DEVICES; GROWTH; OXIDES
AB Metal electrodes are a universal element of all electronic devices. Conducting SrRuO3 (SRO) epitaxial thin films have been extensively used as electrodes in complex-oxide heterostructures due to good lattice mismatches with perovskite substrates. However, when compared to SRO single crystals, SRO thin films have shown reduced conductivity and Curie temperatures (T-C), which can lead to higher Joule heating and energy loss in the devices. Here, we report that high-quality SRO thin films can be synthesized by controlling the plume dynamics and growth rate of pulsed laser epitaxy (PLE) with real-time optical spectroscopic monitoring. The SRO thin films grown under the kinetically controlled conditions, down to ca. 16 nm in thickness, exhibit both enhanced conductivity and T-C as compared to bulk values, due to their improved stoichiometry and a strain-mediated increase of the bandwidth of Ru 4d electrons. This result provides a direction for enhancing the physical properties of PLE-grown thin films and paves a way to improved device applications. Published by AIP Publishing.
C1 [Thompson, J.; Gruenewald, J. H.; Connell, J. G.; Souri, M.; Seo, S. S. A.] Univ Kentucky, Dept Phys & Astron, Lexington, KY 40506 USA.
[Nichols, J.; Lee, S.; Lee, H. N.] Oak Ridge Natl Lab, Mat Sci & Technol Div, Oak Ridge, TN 37831 USA.
[Ryee, S.; Han, M. J.] Korea Adv Inst Sci & Technol, Dept Phys, Daejeon 305701, South Korea.
[Johnson, J. M.; Hwang, J.] Ohio State Univ, Dept Mat Sci & Engn, 116 W 19Th Ave, Columbus, OH 43212 USA.
[Kim, D. -W.] Ewha Womans Univ, Dept Phys, Seoul 120750, South Korea.
RP Seo, SSA (reprint author), Univ Kentucky, Dept Phys & Astron, Lexington, KY 40506 USA.
EM a.seo@uky.edu
RI LEE, SHINBUHM/A-9494-2011; Lee, Ho Nyung/K-2820-2012; Han, Myung
Joon/H-7104-2012; HWANG, JINWOO/D-1760-2013
OI LEE, SHINBUHM/0000-0002-4907-7362; Lee, Ho Nyung/0000-0002-2180-3975;
Han, Myung Joon/0000-0002-8089-7991;
FU National Science Foundation [DMR-1454200]; Basic Science Research
Program through NRF [2014R1A1A2057202]; KISTI [KSC-2014-C2-046]; U.S.
Department of Energy, Office of Science, Basic Energy Sciences,
Materials Science and Engineering Division
FX We acknowledge the support of the National Science Foundation Grant No.
DMR-1454200 for the sample syntheses and characterizations. S.R. and
M.J.H. were supported by the Basic Science Research Program through NRF
(2014R1A1A2057202), and the computing resource is supported by KISTI
(KSC-2014-C2-046). The XRD measurements performed at ORNL were supported
by the U.S. Department of Energy, Office of Science, Basic Energy
Sciences, Materials Science and Engineering Division.
NR 34
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U1 17
U2 17
PU AMER INST PHYSICS
PI MELVILLE
PA 1305 WALT WHITMAN RD, STE 300, MELVILLE, NY 11747-4501 USA
SN 0003-6951
EI 1077-3118
J9 APPL PHYS LETT
JI Appl. Phys. Lett.
PD OCT 17
PY 2016
VL 109
IS 16
AR 161902
DI 10.1063/1.4964882
PG 5
WC Physics, Applied
SC Physics
GA EA9AT
UT WOS:000386933200011
ER
PT J
AU Yu, C
Ren, Y
Cui, LS
Ma, ZY
Yang, WG
AF Yu, Cun
Ren, Yang
Cui, Lishan
Ma, Zhiyuan
Yang, Wenge
TI Anomalous expansion of Nb nanowires in a NiTi matrix under high pressure
SO APPLIED PHYSICS LETTERS
LA English
DT Article
ID MARTENSITIC-TRANSFORMATION; ELASTIC-CONSTANTS; TRANSITION; MODULUS;
METALS; IRON
AB Under high pressure, materials usually shrink during compression as described by an equation of state. Here, we present the anomalous volume expansion behavior of a one-dimensional Nb nano-wire embedded in a NiTi transforming matrix, while the matrix undergoes a pressure-induced martensitic transformation. The Nb volume expansion depends on the NiTi transition pressure range from the matrix, which is controlled by the shear strain induced by different pressure transmitting media. The transformation-induced interfacial stresses between Nb and NiTi may play a major role in this anomaly. Our discovery sheds new light on the nano-interfacial effect on mechanical anomalies in heterogeneous systems during a pressure-induced phase transition. Published by AIP Publishing.
C1 [Yu, Cun; Cui, Lishan; Ma, Zhiyuan] China Univ Petr, Dept Mat Sci & Engn, Beijing 102249, Peoples R China.
[Yu, Cun] Chinese Acad Sci, Shanghai Inst Appl Phys, Shanghai 201800, Peoples R China.
[Ren, Yang] Argon Natl Lab, Xray Sci Div, Argonne, IL 60439 USA.
[Yang, Wenge] Ctr High Pressure Sci & Technol Adv Res HPSTAR, Shanghai 201203, Peoples R China.
[Yang, Wenge] Carnegie Inst Sci, Geophys Lab, High Pressure Synerget Consortium HPSynC, Argonne, IL 60439 USA.
RP Cui, LS (reprint author), China Univ Petr, Dept Mat Sci & Engn, Beijing 102249, Peoples R China.; Yang, WG (reprint author), Ctr High Pressure Sci & Technol Adv Res HPSTAR, Shanghai 201203, Peoples R China.; Yang, WG (reprint author), Carnegie Inst Sci, Geophys Lab, High Pressure Synerget Consortium HPSynC, Argonne, IL 60439 USA.
EM lscui@cup.edu.cn; yangwg@hpstar.ac.cn
FU National Natural Science Foundation of China (NSFC) [51231008, 11474362,
U1530402]; DOE-NNSA [DE-NA0001974]; DOE-BES [DE-FG02-99ER45775]; NSF;
U.S. Department of Energy, Office of Science, Office of Basic Energy
Sciences [DE-AC02-06CH11357]; [EAR-1128799]; [DE-FG02-94ER14466]
FX The authors acknowledge the support of the National Natural Science
Foundation of China (NSFC) (Grant Nos. 51231008, 11474362, and
U1530402). HPCAT operations are supported by DOE-NNSA under Award
DE-NA0001974 and DOE-BES under Award DE-FG02-99ER45775, with partial
instrumentation funding by NSF. The gas loading was performed at
GeoSoilEnviroCARS, APS, ANL, supported by EAR-1128799 and
DE-FG02-94ER14466. Use of the Advanced Photon Source was supported by
the U.S. Department of Energy, Office of Science, Office of Basic Energy
Sciences, under Contract No. DE-AC02-06CH11357.
NR 13
TC 0
Z9 0
U1 3
U2 3
PU AMER INST PHYSICS
PI MELVILLE
PA 1305 WALT WHITMAN RD, STE 300, MELVILLE, NY 11747-4501 USA
SN 0003-6951
EI 1077-3118
J9 APPL PHYS LETT
JI Appl. Phys. Lett.
PD OCT 17
PY 2016
VL 109
IS 16
AR 161903
DI 10.1063/1.4965117
PG 5
WC Physics, Applied
SC Physics
GA EA9AT
UT WOS:000386933200012
ER
PT J
AU Dumitrescu, PT
Serbyn, M
Scalettar, RT
Vishwanath, A
AF Dumitrescu, Philipp T.
Serbyn, Maksym
Scalettar, Richard T.
Vishwanath, Ashvin
TI Superconductivity and nematic fluctuations in a model of doped FeSe
monolayers: Determinant quantum Monte Carlo study
SO PHYSICAL REVIEW B
LA English
DT Article
ID SINGLE-LAYER FESE; HIGH-TEMPERATURE SUPERCONDUCTIVITY; 2-DIMENSIONAL
HUBBARD-MODEL; T-C; PHASE-DIAGRAM; THIN-FILMS; 65 K; SRTIO3;
ANTIFERROMAGNETISM; BEHAVIOR
AB In contrast to bulk FeSe, which exhibits nematic order and low temperature superconductivity, highly doped FeSe reverses the situation, having high temperature superconductivity appearing alongside a suppression of nematic order. To investigate this phenomenon, we study a minimal electronic model of FeSe, with interactions that enhance nematic fluctuations. This model is sign problem free, and is simulated using determinant quantum Monte Carlo (DQMC). We developed a DQMC algorithm with parallel tempering, which proves to be an efficient source of global updates and allows us to access the region of strong interactions. Over a wide range of intermediate couplings, we observe superconductivity with an extended s-wave order parameter, along with enhanced, but short-ranged, q = (0,0) ferro-orbital (nematic) order. These results are consistent with approximate weak-coupling treatments that predict that nematic fluctuations lead to superconducting pairing. Surprisingly, in the parameter range under study, we do not observe nematic long-range order. Instead, at stronger coupling an unusual insulating phase with q = (pi, pi) antiferro-orbital order appears, which is missed by weak-coupling approximations.
C1 [Dumitrescu, Philipp T.; Serbyn, Maksym; Vishwanath, Ashvin] Univ Calif Berkeley, Dept Phys, Berkeley, CA 94720 USA.
[Scalettar, Richard T.] Univ Calif Davis, Dept Phys, Davis, CA 95616 USA.
[Vishwanath, Ashvin] Lawrence Berkeley Natl Labs, Div Mat Sci, Berkeley, CA 94720 USA.
RP Dumitrescu, PT (reprint author), Univ Calif Berkeley, Dept Phys, Berkeley, CA 94720 USA.
EM philippd@berkeley.edu
FU Gordon and Betty Moore Foundation EPiQS Initiative [GBMF4307]; U.S.
Department of Energy, Office of Science, Office of Basic Energy Sciences
[DE-SC0014671]; Simons Investigator grant
FX We thank S. Gazit for numerous discussions. This research was supported
by the Gordon and Betty Moore Foundation EPiQS Initiative through Grant
No. GBMF4307 (M.S.), the U.S. Department of Energy, Office of Science,
Office of Basic Energy Sciences under Grant No. DE-SC0014671 (R.T.S.),
and a Simons Investigator grant (A.V.).
NR 51
TC 4
Z9 4
U1 7
U2 7
PU AMER PHYSICAL SOC
PI COLLEGE PK
PA ONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA
SN 2469-9950
EI 2469-9969
J9 PHYS REV B
JI Phys. Rev. B
PD OCT 17
PY 2016
VL 94
IS 15
AR 155127
DI 10.1103/PhysRevB.94.155127
PG 8
WC Physics, Condensed Matter
SC Physics
GA DZ8CU
UT WOS:000386097100002
ER
PT J
AU Holleman, J
Bishop, MM
Garcia, C
Winfred, JSRV
Lee, S
Lee, HN
Beekman, C
Manousakis, E
McGill, SA
AF Holleman, Joshua
Bishop, Michael M.
Garcia, Carlos
Winfred, J. S. R. Vellore
Lee, Shinbuhm
Lee, Ho Nyung
Beekman, Christianne
Manousakis, Efstratios
McGill, Stephen A.
TI Evidence for impact ionization in vanadium dioxide
SO PHYSICAL REVIEW B
LA English
DT Article
ID OXIDE INTERFACES; PHASE; VO2; ELECTRONICS
AB Pump-probe optical spectroscopy was used to investigate proposed charge-carrier multiplication via impact ionization in the M-1 insulating phase of VO2. By comparing the transient reflectivities of the film when pumped at less than and then more than twice the band-gap energy, we observed a larger ultrafast response with the higher energy pump color while the film was still transiently in the insulating phase. We additionally identified multiple time scales within the charge dynamics and analyzed how these changed when the pump and probe wavelengths were varied. This experiment provided evidence that a fast carrier multiplication process, i.e., impact ionization, acts efficiently in this prototypical strongly correlated insulator, as was recently predicted by theoretical calculations.
C1 [Holleman, Joshua; Bishop, Michael M.; Garcia, Carlos; Winfred, J. S. R. Vellore; Beekman, Christianne; Manousakis, Efstratios; McGill, Stephen A.] Natl High Magnet Field Lab, 1800 E Paul Dirac Dr, Tallahassee, FL 32310 USA.
[Holleman, Joshua; Garcia, Carlos; Beekman, Christianne; Manousakis, Efstratios] Florida State Univ, Dept Phys, Tallahassee, FL 32306 USA.
[Lee, Shinbuhm; Lee, Ho Nyung] Oak Ridge Natl Lab, Div Mat Sci & Technol, Oak Ridge, TN 37831 USA.
RP McGill, SA (reprint author), Natl High Magnet Field Lab, 1800 E Paul Dirac Dr, Tallahassee, FL 32310 USA.
EM mcgill@magnet.fsu.edu
RI LEE, SHINBUHM/A-9494-2011
OI LEE, SHINBUHM/0000-0002-4907-7362
FU NSF [DMR-1229217]; U.S. Department of Energy, Office of Science, Basic
Energy Sciences, Materials Sciences and Engineering Division; National
Science Foundation [DMR-1157490]; State of Florida
FX S.M. acknowledges support from the NSF (DMR-1229217). S.L. and H.N.L.
were supported by the U.S. Department of Energy, Office of Science,
Basic Energy Sciences, Materials Sciences and Engineering Division. A
portion of this work was performed at the National High Magnetic Field
Laboratory, which was supported by National Science Foundation
Cooperative Agreement No. DMR-1157490 and the State of Florida.
NR 31
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U1 19
U2 19
PU AMER PHYSICAL SOC
PI COLLEGE PK
PA ONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA
SN 2469-9950
EI 2469-9969
J9 PHYS REV B
JI Phys. Rev. B
PD OCT 17
PY 2016
VL 94
IS 15
AR 155129
DI 10.1103/PhysRevB.94.155129
PG 7
WC Physics, Condensed Matter
SC Physics
GA DZ8CU
UT WOS:000386097100004
ER
PT J
AU Pan, W
Baldwin, KW
West, KW
Pfeiffer, LN
Tsui, DC
AF Pan, W.
Baldwin, K. W.
West, K. W.
Pfeiffer, L. N.
Tsui, D. C.
TI Antilevitation of Landau levels in vanishing magnetic fields
SO PHYSICAL REVIEW B
LA English
DT Article
ID QUANTIZED HALL CONDUCTANCE; 2-DIMENSIONAL ELECTRON-GAS; GLOBAL
PHASE-DIAGRAM; DELOCALIZED STATES; EXTENDED STATES; 2 DIMENSIONS;
QUANTUM; LEVITATION; LOCALIZATION; MAGNETOTRANSPORT
AB We report in this Rapid Communication an antilevitation behavior of Landau levels in vanishing magnetic fields in a high quality heterojunction insulated-gated field-effect transistor. We found, in the Landau fan diagram of electron density versus magnetic field, the positions of the magnetoresistance minima at Landau-level fillings nu = 4-6 move below the "traditional" Landau-level line to lower electron densities. Moreover, the even and odd filling factors show quantitatively different behaviors in antilevitation, suggesting that the exchange interactions may be important.
C1 [Pan, W.] Sandia Natl Labs, Albuquerque, NM 87185 USA.
[Baldwin, K. W.; West, K. W.; Pfeiffer, L. N.; Tsui, D. C.] Princeton Univ, Princeton, NJ 08544 USA.
RP Pan, W (reprint author), Sandia Natl Labs, Albuquerque, NM 87185 USA.
FU U.S. Department of Energy, Office of Science, Basic Energy Sciences,
Materials Sciences and Engineering Division; US Department of Energy's
National Nuclear Security Administration [DE-AC04-94AL85000]; Gordon and
Betty Moore Foundation through the EPiQS initiative [GBMF4420]; National
Science Foundation MRSEC Grant [DMR-1420541]
FX We thank X. R. Wang and K. Yang for very helpful discussions. This work
was supported by the U.S. Department of Energy, Office of Science, Basic
Energy Sciences, Materials Sciences and Engineering Division. Sandia
National Laboratories is a multiprogram laboratory managed and operated
by the Sandia Corporation, a wholly owned subsidiary of the Lockheed
Martin Corporation, for the US Department of Energy's National Nuclear
Security Administration under Contract No. DE-AC04-94AL85000. Sample
growth at Princeton was funded by the Gordon and Betty Moore Foundation
through the EPiQS initiative Grant No. GBMF4420 and by the National
Science Foundation MRSEC Grant No. DMR-1420541.
NR 27
TC 0
Z9 0
U1 3
U2 3
PU AMER PHYSICAL SOC
PI COLLEGE PK
PA ONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA
SN 2469-9950
EI 2469-9969
J9 PHYS REV B
JI Phys. Rev. B
PD OCT 17
PY 2016
VL 94
IS 16
AR 161303
DI 10.1103/PhysRevB.94.161303
PG 4
WC Physics, Condensed Matter
SC Physics
GA DZ9AP
UT WOS:000386165700002
ER
PT J
AU Wang, Z
Tao, J
Yu, LP
Guo, HW
Chen, LN
Han, MG
Wu, LJ
Xin, HL
Kisslinger, K
Plummer, EW
Zhang, JD
Zhu, YM
AF Wang, Zhen
Tao, Jing
Yu, Liping
Guo, Hangwen
Chen, Lina
Han, Myung-Geun
Wu, Lijun
Xin, Huolin
Kisslinger, Kim
Plummer, E. W.
Zhang, Jiandi
Zhu, Yimei
TI Anomalously deep polarization in SrTiO3 (001) interfaced with an
epitaxial ultrathin manganite film
SO PHYSICAL REVIEW B
LA English
DT Article
ID 2D ELECTRON-GAS; OXIDE INTERFACES; ATOMIC-SCALE; FERROELECTRIC-FILMS;
SURFACE; PEROVSKITE; RESOLUTION; INSULATOR
AB Using atomically resolved imaging and spectroscopy, we reveal a remarkably deep polarization in nonferroelectric SrTiO3 near its interface with an ultrathin nonmetallic film of La2/3Sr1/3MnO3. Electron holography shows an electric field near the interface in SrTiO3, yielding a surprising spontaneous polarization density of similar to 21 mu C/cm(2). Combining the experimental results with first-principles calculations, we propose that the observed deep polarization is induced by the electric field originating from oxygen vacancies that extend beyond a dozen unit cells from the interface, thus providing important evidence of the role of defects in the emergent interface properties of transition metal oxides.
C1 [Wang, Zhen; Guo, Hangwen; Chen, Lina; Plummer, E. W.; Zhang, Jiandi] Louisiana State Univ, Dept Phys & Astron, Baton Rouge, LA 70803 USA.
[Wang, Zhen; Tao, Jing; Han, Myung-Geun; Wu, Lijun; Xin, Huolin; Kisslinger, Kim; Zhu, Yimei] Brookhaven Natl Lab, Dept Energy Sci & Technol, Upton, NY 11973 USA.
[Yu, Liping] Temple Univ, Dept Phys, Philadelphia, PA 19122 USA.
RP Plummer, EW (reprint author), Louisiana State Univ, Dept Phys & Astron, Baton Rouge, LA 70803 USA.
EM wplummer@phys.lsu.edu; jiandiz@lsu.edu; zhu@bnl.gov
FU U.S. Department of Energy (DOE) [DOE DE-SC0002136]; Materials Science
and Engineering Divisions, Office of Basic Energy Sciences of the U.S.
Department of Energy [DESC0012704]; U.S. National Science Foundation
[CNS-0821794]; University of Colorado
FX The paper is primarily supported by the U.S. Department of Energy (DOE)
under Grant No. DOE DE-SC0002136 (Z.W., H.G., L.C., E.W.P., and J.Z.).
The electron microscopic work done at BNL is sponsored by the Materials
Science and Engineering Divisions, Office of Basic Energy Sciences of
the U.S. Department of Energy under Contract No. DESC0012704 (J.T.,
M.-G.H., L.W., and Y.Z.). The calculations were done with FQ the Janus
supercomputer supported by U.S. National Science Foundation under Grant
No. CNS-0821794 and the University of Colorado (L.Y.). The use of DOE
BES user facilities for the TEM sample preparation at the Center for
Functional Nanomaterials at BNL is also acknowledged (H.X. and K.K.).
NR 52
TC 1
Z9 1
U1 8
U2 8
PU AMER PHYSICAL SOC
PI COLLEGE PK
PA ONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA
SN 2469-9950
EI 2469-9969
J9 PHYS REV B
JI Phys. Rev. B
PD OCT 17
PY 2016
VL 94
IS 15
AR 155307
DI 10.1103/PhysRevB.94.155307
PG 9
WC Physics, Condensed Matter
SC Physics
GA DZ8CU
UT WOS:000386097100007
ER
PT J
AU Wong, A
Ngo, AT
Ulloa, SE
AF Wong, Arturo
Ngo, Anh T.
Ulloa, Sergio E.
TI Magnetic-field-induced mixed-level Kondo effect in two-level systems
SO PHYSICAL REVIEW B
LA English
DT Article
ID NUMERICAL RENORMALIZATION-GROUP; SINGLE-ELECTRON TRANSISTOR; ANDERSON
MODEL; CARBON NANOTUBES; QUANTUM DOTS; ALLOYS
AB We consider a two-orbital impurity system with intra-and interlevel Coulomb repulsion that is coupled to a single conduction channel. This situation can generically occur in multilevel quantum dots or in systems of coupled quantum dots. For finite energy spacing between spin-degenerate orbitals, an in-plane magnetic field drives the system from a local-singlet ground state to a "mixed-level" Kondo regime, where the Zeeman-split levels are degenerate for opposite-spin states. We use the numerical renormalization group approach to fully characterize this mixed-level Kondo state and discuss its properties in terms of the applied Zeeman field, temperature, and system parameters. Under suitable conditions, the total spectral function is shown to develop a Fermi-level resonance, so that the linear conductance of the system peaks at a finite Zeeman field while it decreases as a function of temperature. These features, as well as the local moment and entropy contribution of the impurity system, are commensurate with Kondo physics, which can be studied in suitably tuned quantum dot systems.
C1 [Wong, Arturo; Ulloa, Sergio E.] Ohio Univ, Dept Phys & Astron, Athens, OH 45701 USA.
[Wong, Arturo; Ulloa, Sergio E.] Ohio Univ, Nanoscale & Quantum Phenomena Inst, Athens, OH 45701 USA.
[Wong, Arturo] Univ Nacl Autonoma Mexico, Dept Fis Teor, Ctr Nanociencias & Nanotecnol, Apartado Postal 2681, Ensenada 22800, Baja California, Mexico.
[Ngo, Anh T.] Argonne Natl Lab, Div Mat Sci, 9700 S Cass Ave, Argonne, IL 60439 USA.
RP Wong, A (reprint author), Ohio Univ, Dept Phys & Astron, Athens, OH 45701 USA.; Wong, A (reprint author), Ohio Univ, Nanoscale & Quantum Phenomena Inst, Athens, OH 45701 USA.; Wong, A (reprint author), Univ Nacl Autonoma Mexico, Dept Fis Teor, Ctr Nanociencias & Nanotecnol, Apartado Postal 2681, Ensenada 22800, Baja California, Mexico.
RI Ulloa, Sergio/F-4621-2011
OI Ulloa, Sergio/0000-0002-3091-4984
FU NSF [DMR 1508325]
FX We acknowledge support from NSF Grant No. DMR 1508325 and useful
discussions with A. Kogan and his group at U. Cincinnati.
NR 26
TC 0
Z9 0
U1 4
U2 4
PU AMER PHYSICAL SOC
PI COLLEGE PK
PA ONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA
SN 2469-9950
EI 2469-9969
J9 PHYS REV B
JI Phys. Rev. B
PD OCT 17
PY 2016
VL 94
IS 15
AR 155130
DI 10.1103/PhysRevB.94.155130
PG 8
WC Physics, Condensed Matter
SC Physics
GA DZ8CU
UT WOS:000386097100005
ER
PT J
AU Fotiades, N
Devlin, M
Nelson, RO
Kawano, T
Carroll, JJ
AF Fotiades, N.
Devlin, M.
Nelson, R. O.
Kawano, T.
Carroll, J. J.
TI Feeding of Rh and Ag isomers in fast-neutron-induced reactions
SO PHYSICAL REVIEW C
LA English
DT Article
ID NUCLEAR-DATA SHEETS; HAUSER-FESHBACH; CROSS-SECTIONS; ENERGY REGION;
MODEL; FORMULA; DECAY
AB Background: In (n, n') reactions on stable Ir and Au isotopes in the mass A = 190 region, the experimentally established feeding of the isomers relative to the feeding of the corresponding ground states increases with increasing neutron energy, up to the neutron energy where the (n, 2n) reaction channel opens up, and then decreases.
Purpose: In order to check for similar behavior in the mass A = 100 region, the feeding of isomers and ground states in fast-neutron-induced reactions on stable isotopes in this mass region was studied. This is of especial interest for Rh which can be used as a radiochemical detector.
Methods: Excited states were studied using the (n, n'gamma), (n, 2n gamma), and (n, 3n gamma.) reactions on Rh-103 and Ag-109. A germanium detector array for gamma-ray detection and the broad-spectrum pulsed neutron source of the Los Alamos Neutron Science Center'sWeapons Neutron Research facility were used for the measurement. The energy of the incident neutrons was determined using the time-of-flight technique.
Results: Absolute partial gamma-ray cross sections weremeasured for 57 transitions feeding isomers and ground states in Rh-101,Rh-102,Rh-103 and Ag-107,Ag-108,Ag-109. The feeding of the isomers was found to be very similar in the corresponding reaction channels and it is compared to the feeding determined for the ground states.
Conclusions: The opening of reaction channels at higher neutron energies removes angular momentum from the residual nucleus and reduces the population of the higher-spin isomers relative to the feeding of the lower-spin ground states. Similar behavior was observed in the mass A = 190 region in the feeding of higher-spin isomers, but the reverse behavior was observed in Lu-176 with a lower-spin isomer and a higher-spin ground state.
C1 [Fotiades, N.; Devlin, M.; Nelson, R. O.; Kawano, T.] Los Alamos Natl Lab, Los Alamos, NM 87545 USA.
[Carroll, J. J.] US Army, Res Lab, Adelphi, MD 20783 USA.
RP Fotiades, N (reprint author), Los Alamos Natl Lab, Los Alamos, NM 87545 USA.
EM fotia@lanl.gov
RI Devlin, Matthew/B-5089-2013;
OI Devlin, Matthew/0000-0002-6948-2154; Fotiadis,
Nikolaos/0000-0003-1410-3871
FU US Department of Energy (DOE) [DE-AC52-06NA25396]; DOE
[DE-AC52-06NA25396]; US Army Research Laboratory [W911QX09D0016-0003]
FX This work was performed under the auspices of the US Department of
Energy (DOE) under Contract No. DE-AC52-06NA25396. This work has
benefited from use of the LANSCE accelerator facility supported under
DOE Contract No. DE-AC52-06NA25396. The enriched 109Ag target
was provided by Ecopulse, Inc. under US Army Research Laboratory
Contract No. W911QX09D0016-0003.
NR 44
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U1 1
U2 1
PU AMER PHYSICAL SOC
PI COLLEGE PK
PA ONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA
SN 2469-9985
EI 2469-9993
J9 PHYS REV C
JI Phys. Rev. C
PD OCT 17
PY 2016
VL 94
IS 4
AR 044608
DI 10.1103/PhysRevC.94.044608
PG 9
WC Physics, Nuclear
SC Physics
GA DZ9CE
UT WOS:000386170000005
ER
PT J
AU Hagen, G
Jansen, GR
Papenbrock, T
AF Hagen, G.
Jansen, G. R.
Papenbrock, T.
TI Structure of Ni-78 from First-Principles Computations
SO PHYSICAL REVIEW LETTERS
LA English
DT Article
ID COUPLED-CLUSTER THEORY; EXCITATION-ENERGIES; NUCLEAR-FORCES; STATES;
PARTICLE; EXPANSIONS; SCATTERING; SYSTEMS
AB Doubly magic nuclei have a simple structure and are the cornerstones for entire regions of the nuclear chart. Theoretical insights into the supposedly doubly magic Ni-78 and its neighbors are challenging because of the extreme neutron-to-proton ratio and the proximity of the continuum. We predict the J(pi) = 2(1)(+) state in Ni-78 from a correlation with the J(pi) = 2(1)(+) state in Ca-48 using chiral nucleon-nucleon and three-nucleon interactions. Our results confirm that Ni-78 is doubly magic, and the predicted low-lying states of Ni-79,Ni-80 open the way for shell-model studies of many more rare isotopes.
C1 [Hagen, G.; Jansen, G. R.; Papenbrock, T.] Oak Ridge Natl Lab, Div Phys, Oak Ridge, TN 37831 USA.
[Hagen, G.; Papenbrock, T.] Univ Tennessee, Dept Phys & Astron, Knoxville, TN 37996 USA.
[Jansen, G. R.] Oak Ridge Natl Lab, Natl Ctr Computat Sci, Oak Ridge, TN 37831 USA.
RP Hagen, G (reprint author), Oak Ridge Natl Lab, Div Phys, Oak Ridge, TN 37831 USA.; Hagen, G (reprint author), Univ Tennessee, Dept Phys & Astron, Knoxville, TN 37996 USA.
OI Hagen, Gaute/0000-0001-6019-1687
FU Office of Nuclear Physics, U.S. Department of Energy [DE-FG02-96ER40963,
DE-SC0008499]; Oak Ridge National Laboratory (ORNL); Office of Science
of the Department of Energy [DE-AC05-00OR22725]; U.S. Department of
Energy [DE-AC05-00OR22725]
FX We thank Kai Hebeler for providing us with matrix elements in Jacobi
coordinates for the three-nucleon interaction at next-to-next-to-leading
order. This work was supported by the Office of Nuclear Physics, U.S.
Department of Energy, under Grants No. DE-FG02-96ER40963 and No.
DE-SC0008499 (NUCLEI SciDAC Collaboration), and the Field Work Proposal
ERKBP57 at Oak Ridge National Laboratory (ORNL). Computer time was
provided by the Innovative and Novel Computational Impact on Theory and
Experiment (INCITE) program. This research used resources of the Oak
Ridge Leadership Computing Facility located at ORNL, which is supported
by the Office of Science of the Department of Energy under Contract No.
DE-AC05-00OR22725.; This manuscript has been authored by UT-Battelle,
LLC under Contract No. DE-AC05-00OR22725 with the U.S. Department of
Energy. The U.S. Government retains a nonexclusive, paid-up,
irrevocable, world-wide license to publish or reproduce the published
form of this manuscript, or allow others to do so, for U.S. Government
purposes. The views and conclusions contained herein are those of the
authors and should not be interpreted as necessarily representing the
official policies or endorsements, either expressed or implied, of the
U.S. Government or any U.S. Government agency. The Department of Energy
will provide public access to these results of federally sponsored
research in accordance with the DOE Public Access Plan.
NR 85
TC 1
Z9 1
U1 9
U2 9
PU AMER PHYSICAL SOC
PI COLLEGE PK
PA ONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA
SN 0031-9007
EI 1079-7114
J9 PHYS REV LETT
JI Phys. Rev. Lett.
PD OCT 17
PY 2016
VL 117
IS 17
AR 172501
DI 10.1103/PhysRevLett.117.172501
PG 7
WC Physics, Multidisciplinary
SC Physics
GA EA1ZT
UT WOS:000386391500001
PM 27824459
ER
PT J
AU Chen, YF
Jamshidi, R
White, K
Cinar, S
Gallegos, E
Hashemi, N
Montazami, R
AF Chen, Yuanfen
Jamshidi, Reihaneh
White, Kathryn
Cinar, Simge
Gallegos, Emma
Hashemi, Nastaran
Montazami, Reza
TI Physical-Chemical Hybrid Transiency: A Fully Transient Li-Ion Battery
Based on Insoluble Active Materials
SO JOURNAL OF POLYMER SCIENCE PART B-POLYMER PHYSICS
LA English
DT Article
DE colloids; degradation; hybrid transiency; Li-ion battery;
physical-chemical transiency; swelling; transient batteries; transient
electronics
ID ELECTRONICS; DEVICES; BIOELECTRONICS; GREEN
AB Transient Li-ion batteries based on polymeric constituents are presented, exhibiting a twofold increase in the potential and approximately three orders of magnitude faster transiency rate compared to other transient systems reported in the literature. The battery takes advantage of a close variation of the active materials used in conventional Li-ion batteries and can achieve and maintain a potential of >2.5 V. All materials are deposited form polymer-based emulsions and the transiency is achieved through a hybrid approach of redispersion of insoluble, and dissolution of soluble components in approximately 30 min. The presented proof of concept has paramount potentials in military and hardware security applications. (C) 2016 Wiley Periodicals, Inc.
C1 [Chen, Yuanfen; Jamshidi, Reihaneh; White, Kathryn; Cinar, Simge; Gallegos, Emma; Hashemi, Nastaran; Montazami, Reza] Iowa State Univ, Dept Mech Engn, Ames, IA 50011 USA.
[Montazami, Reza] US DOE, Ames Natl Lab, Ames, IA 50011 USA.
RP Montazami, R (reprint author), Iowa State Univ, Dept Mech Engn, Ames, IA 50011 USA.; Montazami, R (reprint author), US DOE, Ames Natl Lab, Ames, IA 50011 USA.
EM reza@iastate.edu
OI Cinar, Simge/0000-0003-3098-2888; Hashemi, Nicole/0000-0001-8921-7588;
Montazami, Reza/0000-0002-8827-0026
FU Iowa State University PIIR (Presidential Initiative for
Interdisciplinary Research) grant
FX This work was supported in part by Iowa State University PIIR
(Presidential Initiative for Interdisciplinary Research) grant. R.
Montazami thanks Ashley Christopherson for her help and contribution to
this research paper by providing scientific illustrations.
NR 20
TC 1
Z9 1
U1 3
U2 3
PU WILEY-BLACKWELL
PI HOBOKEN
PA 111 RIVER ST, HOBOKEN 07030-5774, NJ USA
SN 0887-6266
EI 1099-0488
J9 J POLYM SCI POL PHYS
JI J. Polym. Sci. Pt. B-Polym. Phys.
PD OCT 15
PY 2016
VL 54
IS 20
BP 2021
EP 2027
DI 10.1002/polb.24113
PG 7
WC Polymer Science
SC Polymer Science
GA DW4NK
UT WOS:000383619800001
ER
PT J
AU Powell, KM
Kim, JS
Cole, WJ
Kapoor, K
Mojica, JL
Hedengren, JD
Edgar, TF
AF Powell, Kody M.
Kim, Jong Suk
Cole, Wesley J.
Kapoor, Kriti
Mojica, Jose L.
Hedengren, John D.
Edgar, Thomas F.
TI Thermal energy storage to minimize cost and improve efficiency of a
polygeneration district energy system in a real-time electricity market
SO ENERGY
LA English
DT Article
DE Polygeneration; Thermal energy storage; Combined heat and power; Dynamic
optimization; District energy systems
ID COMBINED HEAT; POWER-SYSTEMS; SMART GRIDS; OPTIMIZATION; PLANT;
PERFORMANCE; OPERATION; DISPATCH; DESIGN; BUILDINGS
AB District energy systems can produce low-cost utilities for large energy networks, but can also be a resource for the electric grid by their ability to ramp production or to store thermal energy by responding to real-time market signals. In this work, dynamic optimization exploits the flexibility of thermal energy storage by determining optimal times to store and extract excess energy. This concept is applied to a polygeneration distributed energy system with combined heat and power, district heating, district cooling, and chilled water thermal energy storage. The system is a university campus responsible for meeting the energy needs of tens of thousands of people. The objective for the dynamic optimization problem is to minimize cost over a 24-h period while meeting multiple loads in real time. The paper presents a novel algorithm to solve this dynamic optimization problem with energy storage by decomposing the problem into multiple static mixed-integer nonlinear programming (MINLP) problems. Another innovative feature of this work is the study of a large, complex energy network which includes the interrelations of a wide variety of energy technologies. Results indicate that a cost savings of 16.5% is realized when the system can participate in the wholesale electricity market. (C) 2016 Elsevier Ltd. All rights reserved.
C1 [Powell, Kody M.] Univ Utah, Dept Chem Engn, 50 S Cent Campus Dr, Salt Lake City, UT 84112 USA.
[Kim, Jong Suk] Idaho Natl Lab, Idaho Falls, ID USA.
[Cole, Wesley J.] Natl Renewable Energy Lab, Golden, CO USA.
[Kapoor, Kriti] NXP Semicond, San Jose, CA USA.
[Mojica, Jose L.] ExxonMobil, Irving, TX USA.
[Hedengren, John D.] Brigham Young Univ, Dept Chem Engn, Provo, UT 84602 USA.
[Edgar, Thomas F.] Univ Texas Austin, Dept Chem Engn, Austin, TX 78712 USA.
RP Powell, KM (reprint author), Univ Utah, Dept Chem Engn, 50 S Cent Campus Dr, Salt Lake City, UT 84112 USA.
EM kody.powell@utah.edu
FU University of Texas Office of Sustainability
FX The authors thank the University of Texas at Austin Utilities and Energy
Management Group as well as the University of Texas at Austin Office of
Sustainability for access to equipment, data, and technical expertise.
This research work was supported by a grant from the University of Texas
Office of Sustainability.
NR 40
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U1 14
U2 14
PU PERGAMON-ELSEVIER SCIENCE LTD
PI OXFORD
PA THE BOULEVARD, LANGFORD LANE, KIDLINGTON, OXFORD OX5 1GB, ENGLAND
SN 0360-5442
EI 1873-6785
J9 ENERGY
JI Energy
PD OCT 15
PY 2016
VL 113
BP 52
EP 63
DI 10.1016/j.energy.2016.07.009
PG 12
WC Thermodynamics; Energy & Fuels
SC Thermodynamics; Energy & Fuels
GA EA2GJ
UT WOS:000386410500006
ER
PT J
AU Wiser, R
Millstein, D
Mai, T
Macknick, J
Carpenter, A
Cohen, S
Cole, W
Frew, B
Heath, G
AF Wiser, Ryan
Millstein, Dev
Mai, Trieu
Macknick, Jordan
Carpenter, Alberta
Cohen, Stuart
Cole, Wesley
Frew, Bethany
Heath, Garvin
TI The environmental and public health benefits of achieving high
penetrations of solar energy in the United States
SO ENERGY
LA English
DT Article
DE Solar energy; Greenhouse-gases; Air pollution; Public health;
Co-benefits; Water use
ID WIND POWER; NATURAL-GAS; EMISSIONS IMPLICATIONS; US; ELECTRICITY;
GENERATION; CARBON; TECHNOLOGY; MORTALITY; SECTOR
AB We estimate the environmental and public health benefits that may be realized if solar energy cost reductions continue until solar power is competitive across the U.S. without subsidies. Specifically, we model, from 2015 to 2050, solar power induced reductions to greenhouse gas (GHG) emissions, air pollutant emissions, and water usage. To find the incremental benefits of new solar deployment, we compare the difference between two scenarios, one where solar costs have fallen such that solar supplies 14% of the nation's electricity by 2030 and 27% by 2050, and a baseline scenario in which no solar is added after 2014. We monetize benefits, where credible methods exist to do so. We find that under these scenarios, solar power reduces GHG and air pollutants by similar to 10%, from 2015 to 2050, providing a discounted present value of $56-$789 billion (central value of similar to$250 billion, equivalent to similar to 2 c/kWh-solar) in climate benefits and $77-$298 billion (central value of $167 billion, or similar to 1.4 ct/kWh-solar) in air quality and public health benefits. The ranges reflect uncertainty within the literature about the marginal impact of emissions of GHG and air pollutants. Solar power is also found to reduce water withdrawals and consumption by 4% and 9%, respectively, including in many drought-prone states. (C) 2016 Elsevier Ltd. All rights reserved.
C1 [Wiser, Ryan; Millstein, Dev] Lawrence Berkeley Natl Lab, Berkeley, CA 94720 USA.
[Mai, Trieu; Macknick, Jordan; Carpenter, Alberta; Cohen, Stuart; Cole, Wesley; Frew, Bethany; Heath, Garvin] Natl Renewable Energy Lab, Golden, CO USA.
RP Wiser, R (reprint author), Lawrence Berkeley Natl Lab, Berkeley, CA 94720 USA.
EM rhwiser@lbl.gov
FU DOE's Solar Energy Technologies Office, Office of Energy Efficiency and
Renewable Energy [DE-AC02-05CH11231, DE-AC36-08GO28308]
FX For their support of this study, the authors thank the entire U.S.
Department of Energy (DOE) Solar Energy Technologies Office team.
Lawrence Berkeley National Laboratory's contributions to this paper were
funded by DOE's Solar Energy Technologies Office, Office of Energy
Efficiency and Renewable Energy under Contract No. DE-AC02-05CH11231.
National Renewable Energy Laboratory's contributions to this paper were
funded by DOE's Solar Energy Technologies Office, Office of Energy
Efficiency and Renewable Energy under Contract No. DE-AC36-08GO28308.
NR 97
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U2 18
PU PERGAMON-ELSEVIER SCIENCE LTD
PI OXFORD
PA THE BOULEVARD, LANGFORD LANE, KIDLINGTON, OXFORD OX5 1GB, ENGLAND
SN 0360-5442
EI 1873-6785
J9 ENERGY
JI Energy
PD OCT 15
PY 2016
VL 113
BP 472
EP 486
DI 10.1016/j.energy.2016.07.068
PG 15
WC Thermodynamics; Energy & Fuels
SC Thermodynamics; Energy & Fuels
GA EA2GJ
UT WOS:000386410500042
ER
PT J
AU Qiu, R
Caneau, C
Paskova, T
AF Qiu, Roger
Caneau, Catherine
Paskova, Tania
TI Preface
SO JOURNAL OF CRYSTAL GROWTH
LA English
DT Editorial Material
C1 [Qiu, Roger] Lawrence Livermore Natl Lab, Livermore, CA 94550 USA.
[Caneau, Catherine] Corning Inc, Corning, NY 14831 USA.
[Paskova, Tania] North Carolina State Univ, Raleigh, NC 27695 USA.
RP Qiu, R (reprint author), Lawrence Livermore Natl Lab, Livermore, CA 94550 USA.
NR 0
TC 0
Z9 0
U1 1
U2 1
PU ELSEVIER SCIENCE BV
PI AMSTERDAM
PA PO BOX 211, 1000 AE AMSTERDAM, NETHERLANDS
SN 0022-0248
EI 1873-5002
J9 J CRYST GROWTH
JI J. Cryst. Growth
PD OCT 15
PY 2016
VL 452
BP VIII
EP VIII
DI 10.1016/S0022-0248(16)30490-0
PG 1
WC Crystallography; Materials Science, Multidisciplinary; Physics, Applied
SC Crystallography; Materials Science; Physics
GA EA2HT
UT WOS:000386414100001
ER
PT J
AU Chen, C
Zhang, XT
Krishna, L
Kendrick, C
Shang, SL
Toberer, E
Liu, ZK
Tamboli, A
Redwing, JM
AF Chen, Chen
Zhang, Xiaotian
Krishna, Lakshmi
Kendrick, Chito
Shang, Shun-Li
Toberer, Eric
Liu, Zi-Kui
Tamboli, Adele
Redwing, Joan M.
TI Synthesis, characterization and chemical stability of silicon
dichalcogenides, Si(SexS1-x)(2)
SO JOURNAL OF CRYSTAL GROWTH
LA English
DT Article; Proceedings Paper
CT 20th American Conference on Crystal Growth and Epitaxy (ACCGE) / 17th
Biennial Workshop on Organometallic Vapor Phase Epitaxy (OMVPE) / 2nd 2D
Electronic Materials Symposium
CY AUG 02-07, 2015
CL MT
DE Characterization; Computer simulation; Growth from melt; Sulfides; Solar
cells
ID TOTAL-ENERGY CALCULATIONS; WAVE BASIS-SET; GLASSES; SISE2; CRYSTALLINE;
DISELENIDE; EFFICIENCY; DISULFIDE
AB Silicon dichalcogenides have an intriguing crystal structure consisting of long tetrahedral chains held together by van der Waals forces but the electronic and optical properties have been less explored. In the present work, bulk SiSe2, SiS2, and Si(SexS1-x)(2) were synthesized by the congruent melt growth method and characterized by Raman spectroscopy, X-ray Diffraction and UV/visible/IR transmission measurements supported by first-principles calculations. First-principles calculations reveal a nearly linear decrease of band gap energy in Si(SexS1-x)(2) with increasing Se content, i.e., from SiS2 to SiSe2 which corresponds with a blue-shift in the transmission spectra from bulk SiSe2 to Si(Se0.6S0.4)(2), and to SiS2. Air stability tests demonstrate the formation of toxic H2Se/H2S gas from sample oxidation at room temperature upon exposure to ambient air, and great care should be paid when handling these materials. (C) 2016 Elsevier B.V. All rights reserved.
C1 [Chen, Chen; Zhang, Xiaotian; Shang, Shun-Li; Liu, Zi-Kui; Redwing, Joan M.] Penn State Univ, Mat Res Inst, Dept Mat Sci & Engn, University Pk, PA 16802 USA.
[Krishna, Lakshmi; Toberer, Eric] Colorado Sch Mines, Dept Phys, Golden, CO 80401 USA.
[Kendrick, Chito] Michigan Technol Univ, Dept Elect & Comp Engn, Houghton, MI 49931 USA.
[Toberer, Eric; Tamboli, Adele] Natl Renewable Energy Lab, Natl Ctr Photovolta, Golden, CO 80404 USA.
RP Redwing, JM (reprint author), Penn State Univ, Mat Res Inst, Dept Mat Sci & Engn, University Pk, PA 16802 USA.
EM jmr31@psu.edu
RI Shang, Shun-Li/A-6564-2009; Liu, Zi-Kui/A-8196-2009
OI Shang, Shun-Li/0000-0002-6524-8897; Liu, Zi-Kui/0000-0003-3346-3696
NR 30
TC 2
Z9 2
U1 13
U2 13
PU ELSEVIER SCIENCE BV
PI AMSTERDAM
PA PO BOX 211, 1000 AE AMSTERDAM, NETHERLANDS
SN 0022-0248
EI 1873-5002
J9 J CRYST GROWTH
JI J. Cryst. Growth
PD OCT 15
PY 2016
VL 452
BP 151
EP 157
DI 10.1016/j.jcrysgro.2015.12.005
PG 7
WC Crystallography; Materials Science, Multidisciplinary; Physics, Applied
SC Crystallography; Materials Science; Physics
GA EA2HT
UT WOS:000386414100030
ER
PT J
AU McMahon, WE
Warren, EL
Kibbler, AE
France, RM
Norman, AG
Reedy, RC
Olson, JM
Tamboli, AC
Stradins, P
AF McMahon, William E.
Warren, Emily L.
Kibbler, Alan E.
France, Ryan M.
Norman, Andrew G.
Reedy, Robert C.
Olson, Jerry M.
Tamboli, Adele C.
Stradins, Paul
TI Surfaces and interfaces governing the OMVPE growth of APD-free GaP on
AsH3-cleaned vicinal Si(100)
SO JOURNAL OF CRYSTAL GROWTH
LA English
DT Article; Proceedings Paper
CT 20th American Conference on Crystal Growth and Epitaxy (ACCGE) / 17th
Biennial Workshop on Organometallic Vapor Phase Epitaxy (OMVPE) / 2nd 2D
Electronic Materials Symposium
CY AUG 02-07, 2015
CL MT
DE Nucleation; Surface structure; Organometallic vapor phase epitaxy;
Semiconducting silicon; Semiconducting III-V materials; Solar cells
AB Direct growth of GaP on Si enables the integration of III-V and Si optoelectronic devices for a wide variety of applications, and has therefore been the subject of much research for many decades. Most of this effort has been directed toward overcoming the two main technical challenges: 1) removing atmospheric oxygen and carbon contamination and 2) establishing the conditions needed for "APD-free" III-V epitaxy (i.e., without antiphase domains). We have developed an OMVPE process for APD-free GaP growth on Si which overcomes both challenges by using AsH3 to clean and prepare the Si surface in situ at a relatively low temperature. This process is based upon a very brief "AsH3-cleaning" step which simultaneously removes atmospheric contamination (thereby eliminating the need for Si regrowth) and creates a single domain As-terminated Si surface. Here we discuss the key process steps using results from a suite of analysis tools. Published by Elsevier B.V.
C1 [McMahon, William E.; Warren, Emily L.; Kibbler, Alan E.; France, Ryan M.; Norman, Andrew G.; Reedy, Robert C.; Olson, Jerry M.; Tamboli, Adele C.; Stradins, Paul] Natl Renewable Energy Lab, Golden, CO 80401 USA.
RP McMahon, WE (reprint author), Natl Renewable Energy Lab, Golden, CO 80401 USA.
EM bill.mcmahon@nrel.gov
RI Norman, Andrew/F-1859-2010
OI Norman, Andrew/0000-0001-6368-521X
NR 13
TC 0
Z9 0
U1 1
U2 1
PU ELSEVIER SCIENCE BV
PI AMSTERDAM
PA PO BOX 211, 1000 AE AMSTERDAM, NETHERLANDS
SN 0022-0248
EI 1873-5002
J9 J CRYST GROWTH
JI J. Cryst. Growth
PD OCT 15
PY 2016
VL 452
BP 235
EP 239
DI 10.1016/j.jcrysgro.2016.05.014
PG 5
WC Crystallography; Materials Science, Multidisciplinary; Physics, Applied
SC Crystallography; Materials Science; Physics
GA EA2HT
UT WOS:000386414100044
ER
PT J
AU Zhou, YC
McGillick, BE
Teng, YHG
Haranahalli, K
Ojima, I
Swaminathan, S
Rizzo, RC
AF Zhou, Yuchen
McGillick, Brian E.
Teng, Yu-Han Gary
Haranahalli, Krupanandan
Ojima, Iwao
Swaminathan, Subramanyam
Rizzo, Robert C.
TI Identification of small molecule inhibitors of botulinum neurotoxin
serotype E via footprint similarity
SO BIOORGANIC & MEDICINAL CHEMISTRY
LA English
DT Article
DE Botulinum neurotoxin; BoNT/E; Docking; Virtual screening; DOCK;
Footprint similarity; Scoring functions; Molecular dynamics
ID EFFICIENT GENERATION; TARGETING HIVGP41; AM1-BCC MODEL; BINDING-SITE;
DOCK 6; SUBSTRATE; METALLOPROTEASE; FLEXIBILITY; RESISTANCE; CHEMISTRY
AB Botulinum neurotoxins (BoNT) are among the most poisonous substances known, and of the 7 serotypes (A-G) identified thus far at least 4 can cause death in humans. The goal of this work was identification of inhibitors that specifically target the light chain catalytic site of the highly pathogenic but lesser-studied E serotype (BoNT/E). Large-scale computational screening, employing the program DOCK, was used to perform atomic-level docking of 1.4 million small molecules to prioritize those making favorable interactions with the BoNT/E site. In particular, 'footprint similarity' (FPS) scoring was used to identify compounds that could potentially mimic features on the known substrate tetrapeptide RIME. Among 92 compounds purchased and experimentally tested, compound C562-1101 emerged as the most promising hit with an apparent IC50 value three-fold more potent than that of the first reported BoNT/E small molecule inhibitor NSC-77053. Additional analysis showed the predicted binding pose of C562-1101 was geometrically and energetically stable over an ensemble of structures generated by molecular dynamic simulations and that many of the intended interactions seen with RIME were maintained. Several analogs were also computationally designed and predicted to have further molecular mimicry thereby demonstrating the potential utility of footprint-based scoring protocols to help guide hit refinement. (C) 2016 Elsevier Ltd. All rights reserved.
C1 [Zhou, Yuchen; Rizzo, Robert C.] SUNY Stony Brook, Dept Appl Math & Stat, Stony Brook, NY 11794 USA.
[McGillick, Brian E.] SUNY Stony Brook, Grad Program Biochem & Struct Biol, Stony Brook, NY 11794 USA.
[Teng, Yu-Han Gary; Ojima, Iwao; Rizzo, Robert C.] SUNY Stony Brook, Inst Chem Biol & Drug Discovery, Stony Brook, NY 11794 USA.
[Teng, Yu-Han Gary; Haranahalli, Krupanandan; Ojima, Iwao] SUNY Stony Brook, Dept Chem, Stony Brook, NY 11794 USA.
[McGillick, Brian E.; Swaminathan, Subramanyam] Brookhaven Natl Lab, Dept Biol, Upton, NY 11973 USA.
[Rizzo, Robert C.] SUNY Stony Brook, Laufer Ctr Phys & Quantitat Biol, Stony Brook, NY 11794 USA.
RP Rizzo, RC (reprint author), SUNY Stony Brook, Dept Appl Math & Stat, Stony Brook, NY 11794 USA.; Rizzo, RC (reprint author), SUNY Stony Brook, Inst Chem Biol & Drug Discovery, Stony Brook, NY 11794 USA.; Rizzo, RC (reprint author), SUNY Stony Brook, Laufer Ctr Phys & Quantitat Biol, Stony Brook, NY 11794 USA.
EM rizzorc@gmail.com
FU Defense Threat Reduction Agency (DTRA), Department of Defense
[B0742081]; U.S. Department of Energy [DE-ACO2-98CH10886]; State of New
York
FX We thank Dr. William J. Allen for assistance with virtual screening
setups, and Drs. Desigan Kumaran, Subramaniam Eswaramoorthy, Natasha
Nesbitt, and Peter Tonge for helpful discussions. This work was funded
in part through a grant from the Defense Threat Reduction Agency (DTRA),
Department of Defense (B0742081 to S.S.). Research utilized resources at
the New York Center for Computational Sciences at Stony Brook
University/Brookhaven National Laboratory which is supported by the U.S.
Department of Energy under Contract No. DE-ACO2-98CH10886 and by the
State of New York.
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PI OXFORD
PA THE BOULEVARD, LANGFORD LANE, KIDLINGTON, OXFORD OX5 1GB, ENGLAND
SN 0968-0896
EI 1464-3391
J9 BIOORGAN MED CHEM
JI Bioorg. Med. Chem.
PD OCT 15
PY 2016
VL 24
IS 20
BP 4875
EP 4889
DI 10.1016/j.bmc.2016.07.031
PG 15
WC Biochemistry & Molecular Biology; Chemistry, Medicinal; Chemistry,
Organic
SC Biochemistry & Molecular Biology; Pharmacology & Pharmacy; Chemistry
GA DZ5MI
UT WOS:000385905800013
PM 27543389
ER
PT J
AU Evangelista, W
Weir, RL
Ellingson, SR
Harris, JB
Kapoor, K
Smith, JC
Baudry, J
AF Evangelista, Wilfredo
Weir, Rebecca L.
Ellingson, Sally R.
Harris, Jason B.
Kapoor, Karan
Smith, Jeremy C.
Baudry, Jerome
TI Ensemble-based docking: From hit discovery to metabolism and toxicity
predictions
SO BIOORGANIC & MEDICINAL CHEMISTRY
LA English
DT Article
DE Drug discovery; Docking; Computational drug discovery; Toxicity; Hit
discovery; Lead discovery
AB This paper describes and illustrates the use of ensemble-based docking, i.e., using a collection of protein structures in docking calculations for hit discovery, the exploration of biochemical pathways and toxicity prediction of drug candidates. We describe the computational engineering work necessary to enable large ensemble docking campaigns on supercomputers. We show examples where ensemble-based docking has significantly increased the number and the diversity of validated drug candidates. Finally, we illustrate how ensemble-based docking can be extended beyond hit discovery and toward providing a structural basis for the prediction of metabolism and off-target binding relevant to pre-clinical and clinical trials. (C) 2016 Elsevier Ltd. All rights reserved.
C1 [Evangelista, Wilfredo; Weir, Rebecca L.; Smith, Jeremy C.; Baudry, Jerome] Univ Tennessee, Dept Biochem & Cellular & Mol Biol, Knoxville, TN 37996 USA.
[Evangelista, Wilfredo; Weir, Rebecca L.; Ellingson, Sally R.; Harris, Jason B.; Kapoor, Karan; Smith, Jeremy C.; Baudry, Jerome] Oak Ridge Natl Lab, UT ORNL Ctr Mol Biophys, Oak Ridge, TN 37831 USA.
[Ellingson, Sally R.; Harris, Jason B.; Kapoor, Karan; Smith, Jeremy C.; Baudry, Jerome] Univ Tennessee, Genome Sci & Technol, Knoxville, TN 37996 USA.
[Ellingson, Sally R.] Univ Kentucky, Coll Med, Div Biomed Informat, Lexington, KY USA.
[Ellingson, Sally R.] Markey Canc Ctr, Canc Res Informat, Lexington, KY USA.
[Ellingson, Sally R.] Univ Kentucky, Lexington, KY USA.
[Harris, Jason B.] Natl Ctr Computat Toxicol Res, Res Triangle Pk, NC USA.
[Harris, Jason B.] Univ N Carolina, Chapel Hill, NC USA.
[Kapoor, Karan] Georgetown Univ, Washington, DC USA.
RP Smith, JC; Baudry, J (reprint author), Univ Tennessee, Dept Biochem & Cellular & Mol Biol, Knoxville, TN 37996 USA.; Smith, JC; Baudry, J (reprint author), Oak Ridge Natl Lab, UT ORNL Ctr Mol Biophys, Oak Ridge, TN 37831 USA.; Smith, JC; Baudry, J (reprint author), Univ Tennessee, Genome Sci & Technol, Knoxville, TN 37996 USA.
EM smithjc@ornl.gov; jbaudry@utk.edu
RI smith, jeremy/B-7287-2012
OI smith, jeremy/0000-0002-2978-3227
FU University of Tennessee Governor Chair program; Department of
Biochemistry and Cellular and Molecular Biology; National Institutes of
Health [1R43HL11426, 1KL2RR031974]; Department of Energy for the
development of VinaMPI
FX The results presented here describe the work performed computationally
by laboratories in the UT/ORNL Center for Molecular Biophysics. We
express our profound gratitude to our experimental collaborators
(co-authors on the respective publications) who have performed the
experimental work on two of these projects: the Center for Environmental
Biotechnology at the University of Tennessee for the PCB-30
estrogenization pathway project, and Shifa Biomedical and the laboratory
of Dr. Cynthia Peterson at the University of Tennessee for the FXa:FVa
project. This work was financially supported by the University of
Tennessee Governor Chair program for J.C.S. and by a start up grant from
the Department of Biochemistry and Cellular and Molecular Biology to
J.B.; as well as by the National Institutes of Health 1R43HL11426 for
the FXa:FVa project to J.B., and by the National Institutes of Health
1KL2RR031974 and the Department of Energy for the development of VinaMPI
to J.B. and J.C.S.
NR 11
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PI OXFORD
PA THE BOULEVARD, LANGFORD LANE, KIDLINGTON, OXFORD OX5 1GB, ENGLAND
SN 0968-0896
EI 1464-3391
J9 BIOORGAN MED CHEM
JI Bioorg. Med. Chem.
PD OCT 15
PY 2016
VL 24
IS 20
BP 4928
EP 4935
DI 10.1016/j.bmc.2016.07.064
PG 8
WC Biochemistry & Molecular Biology; Chemistry, Medicinal; Chemistry,
Organic
SC Biochemistry & Molecular Biology; Pharmacology & Pharmacy; Chemistry
GA DZ5MI
UT WOS:000385905800018
PM 27543390
ER
PT J
AU Sharma, I
Dong, J
Malikopoulos, AA
Street, M
Ostrowski, J
Kuruganti, T
Jackson, R
AF Sharma, Isha
Dong, Jin
Malikopoulos, Andreas A.
Street, Michael
Ostrowski, Jim
Kuruganti, Teja
Jackson, Roderick
TI A modeling framework for optimal energy management of a residential
building
SO ENERGY AND BUILDINGS
LA English
DT Article
DE Microgrid; Model predictive control (MPC); Demand response;
Optimization; Energy hub; Residential building; Energy storage system;
Energy management system; Mathematical modeling
ID PREDICTIVE CONTROL; SYSTEM
AB Residential buildings are currently equipped with energy production facilities, e.g., solar rooftops and batteries, which in conjunction with smart meters, can function as smart energy hubs coordinating the loads and the resources in an optimal manner. This paper presents a mathematical model for the optimal energy management of a residential building and proposes a centralized energy management system (CEMS) framework for off-grid operation. The model of each component of the hub is integrated within the CEMS. The optimal decisions are determined in real-time by considering these models with realistic parameter settings and customer preferences. Model predictive control (MPC) is used to adapt the optimal decisions on a receding horizon to account for the deviations in the system inputs. Simulation results are presented to demonstrate the feasibility and effectiveness of the proposed CEMS framework. Results show that the proposed CEMS can reduce the energy cost and energy consumption of the customers by approximately 17% and 8%, respectively, over a day. Using the proposed CEMS, the total charging cycles of the ESS were reduced by more than 50% in a day. Published by Elsevier B.V.
C1 [Sharma, Isha; Malikopoulos, Andreas A.; Kuruganti, Teja; Jackson, Roderick] Oak Ridge Natl Lab, One Bethel Valley Rd, Oak Ridge, TN 37831 USA.
[Dong, Jin; Ostrowski, Jim] Univ Tennessee, Knoxville, TN 37996 USA.
[Street, Michael] Georgia Inst Technol, North Ave, Atlanta, GA 30332 USA.
RP Sharma, I (reprint author), Oak Ridge Natl Lab, One Bethel Valley Rd, Oak Ridge, TN 37831 USA.
NR 40
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PU ELSEVIER SCIENCE SA
PI LAUSANNE
PA PO BOX 564, 1001 LAUSANNE, SWITZERLAND
SN 0378-7788
EI 1872-6178
J9 ENERG BUILDINGS
JI Energy Build.
PD OCT 15
PY 2016
VL 130
BP 55
EP 63
DI 10.1016/j.enbuild.2016.08.009
PG 9
WC Construction & Building Technology; Energy & Fuels; Engineering, Civil
SC Construction & Building Technology; Energy & Fuels; Engineering
GA DY7QI
UT WOS:000385323900006
ER
PT J
AU Zhang, LL
Ma, YL
Cheng, XQ
Cui, YZ
Guan, T
Gao, YZ
Du, CY
Yin, GP
Lin, F
Nordlund, D
AF Zhang, Lingling
Ma, Yulin
Cheng, Xinqun
Cui, Yingzhi
Guan, Ting
Gao, Yunzhi
Du, Chunyu
Yin, Geping
Lin, Feng
Nordlund, Dennis
TI Degradation mechanism of over-charged LiCoO2/mesocarbon microbeads
battery during shallow depth of discharge cycling
SO JOURNAL OF POWER SOURCES
LA English
DT Article
DE LiCoO2/MCMB battery; Over-charging; Capacity fading mechanism; Long-term
cycling; Lithium dendrites; Reduction and dissolution of cobalt
ID LITHIUM-ION BATTERIES; RAY-ABSORPTION SPECTROSCOPY; ALKYL CARBONATE
SOLUTIONS; LAYERED CATHODE MATERIALS; ELECTROCHEMICAL PROPERTIES;
OVERCHARGE CONDITIONS; CELL SAFETY; ELECTRODES; DEPOSITION; BEHAVIOR
AB LiCoO2/mesocarbon microbeads (MCMB) batteries are over-charged to different voltage (4.4 V, 4.5 V, 4.6 V, and 4.7 V, respectively) for ten times, and then are cycled 1000 times for shallow depth of discharge. The morphology, structure, and electrochemical performance of the electrode materials were studied in detail in order to identify the capacity fading mechanism of over-charged battery after long-term cycling. The cycling performances of LiCoO2/MCMB batteries are gradually aggravated with the increase of over-charging voltage and the degradation mechanism is diverse upon the degree of overcharging. The capacity fading after long-term cycling of battery over-charged to 4.6 V or 4.7 V is mainly attributed to the cathodes. Soft X-ray absorption spectroscopy (XAS) demonstrates that the lower valence state of cobalt exists on the surface of the LiCoO2 after serious over-charging (4.6 V or 4.7 V), and cobalt is dissolved then deposited on the anode according to the result of energy dispersive spectrometry (EDS). However, after shallow over-charging (4.4 V or 4.5 V), the capacity deterioration is proposed as the loss of active lithium, presented by the generation of the SEI film on the anode, which is verified by water washed tests. (C) 2016 Elsevier B.V. All rights reserved.
C1 [Zhang, Lingling; Ma, Yulin; Cheng, Xinqun; Cui, Yingzhi; Guan, Ting; Gao, Yunzhi; Du, Chunyu; Yin, Geping] Harbin Inst Technol, Sch Chem & Chem Engn, MIIT Key Lab Crit Mat Technol New Energy Convers, Harbin 150001, Peoples R China.
[Lin, Feng] Lawrence Berkeley Natl Lab, Environm Energy Technol Div, Berkeley, CA 94720 USA.
[Nordlund, Dennis] SLAC, Stanford Synchrotron Radiat Lightsource, Menlo Pk, CA 94025 USA.
RP Yin, GP (reprint author), Harbin Inst Technol, POB 1247,92 Xidazhi St, Harbin 150001, Peoples R China.
EM yingeping@hit.edu.cn
FU National High Technology Research and Development Program (863 Program)
of China [2012AA110203]; gs2:National Science Foundation of China
[51202047]; U.S. Department of Energy, Office of Science, and Office of
Basic Energy Sciences [DE-AC02-76SF00515]
FX This work was funded by the National High Technology Research and
Development Program (863 Program) of China (No. 2012AA110203) and the
gs2:National Science Foundation of China (No. 51202047). The synchrotron
X-ray portion of this work was carried out at the Stanford Synchrotron
Radiation Lightsource, a Directorate of SLAC National Accelerator
Laboratory and an Office of Science User Facility operated for the U.S.
Department of Energy Office of Science by Stanford University that is
supported by the U.S. Department of Energy, Office of Science, and
Office of Basic Energy Sciences under Contract No. DE-AC02-76SF00515.
NR 40
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U1 65
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PU ELSEVIER SCIENCE BV
PI AMSTERDAM
PA PO BOX 211, 1000 AE AMSTERDAM, NETHERLANDS
SN 0378-7753
EI 1873-2755
J9 J POWER SOURCES
JI J. Power Sources
PD OCT 15
PY 2016
VL 329
BP 255
EP 261
DI 10.1016/j.jpowsour.2016.08.030
PG 7
WC Chemistry, Physical; Electrochemistry; Energy & Fuels; Materials
Science, Multidisciplinary
SC Chemistry; Electrochemistry; Energy & Fuels; Materials Science
GA DY1KB
UT WOS:000384852800028
ER
PT J
AU Jeong, S
Li, XL
Zheng, JM
Yan, PF
Cao, RG
Jung, HJ
Wang, CM
Liu, J
Zhang, JG
AF Jeong, Sookyung
Li, Xiaolin
Zheng, Jianming
Yan, Pengfei
Cao, Ruiguo
Jung, Hee Joon
Wang, Chongmin
Liu, Jun
Zhang, Ji-Guang
TI Hard carbon coated nano-Si/graphite composite as a high performance
anode for Li-ion batteries
SO JOURNAL OF POWER SOURCES
LA English
DT Article
DE Si/graphite composites; Hard carbon coating; Cycling performance; Rate
capability; Lithium ion batteries
ID ELECTROCHEMICAL-BEHAVIOR; 1,3-DIOXOLANE-LICLO4 SOLUTIONS; SILICON
NANOWIRES; GRAPHITE ANODE; LITHIUM; NANOPARTICLES; ELECTRODES; SIZE
AB With the ever-increasing demands for higher energy densities in Li-ion batteries, alternative anodes with higher reversible capacity are required to replace the conventional graphite anode. Here, we demonstrate a cost-effective hydrothermal carbonization approach to prepare a hard carbon coated nano-Si/graphite (HC-nSi/G) composite as a high performance anode for Li-ion batteries. In this hierarchical structured composite, the hard carbon coating not only provides an efficient pathway for electron transfer, but also alleviates the volume variation of Si during charge/discharge processes. The HC-nSi/G composite electrode shows excellent performance, including a high specific capacity of 878.6 mAh g(-1) based on the total weight of composite, good rate performance, and a decent cycling stability, which is, promising for practical applications. (C) 2016 Elsevier B.V. All rights reserved.
C1 [Jeong, Sookyung; Li, Xiaolin; Zheng, Jianming; Cao, Ruiguo; Jung, Hee Joon; Liu, Jun; Zhang, Ji-Guang] Pacific Northwest Natl Lab, 902 Battelle Blvd, Richland, WA 99352 USA.
[Yan, Pengfei; Wang, Chongmin] Pacific Northwest Natl Lab, Environm Mol Sci Lab, Richland, WA 99352 USA.
RP Zhang, JG (reprint author), Pacific Northwest Natl Lab, 902 Battelle Blvd, Richland, WA 99352 USA.
EM Jiguang.zhang@pnnl.gov
RI yan, pengfei/E-4784-2016
OI yan, pengfei/0000-0001-6387-7502
FU Assistant Secretary for Energy Efficiency and Renewable Energy, Office
of Vehicle Technologies, Advanced Battery Materials Research (BMR)
programs of theU.S. Department of Energy (DOE) [DE-AC02-05CH11231,
18769]; DOE's Office of Biological and Environmental Research at Pacific
Northwest National Laboratory (PNNL); DOE [DE-AC05-76RLO1830]
FX This work was supported by the Assistant Secretary for Energy Efficiency
and Renewable Energy, Office of Vehicle Technologies, Advanced Battery
Materials Research (BMR) programs of the U.S. Department of Energy (DOE)
under contract no. DE-AC02-05CH11231, subcontract no. 18769. The SEM/TEM
observations were conducted in the William R. Wiley Environmental
Molecular Sciences Laboratory (EMSL), a national scientific user
facility sponsored by DOE's Office of Biological and Environmental
Research and located at Pacific Northwest National Laboratory (PNNL).
PNNL is operated by Battelle for the DOE under Contract
DE-AC05-76RLO1830. S. Jeong would like to thank Dr. Daiwon Choi and Dr.
Estevez Luis for their useful discussions.
NR 27
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PU ELSEVIER SCIENCE BV
PI AMSTERDAM
PA PO BOX 211, 1000 AE AMSTERDAM, NETHERLANDS
SN 0378-7753
EI 1873-2755
J9 J POWER SOURCES
JI J. Power Sources
PD OCT 15
PY 2016
VL 329
BP 323
EP 329
DI 10.1016/j.jpowsour.2016.08.089
PG 7
WC Chemistry, Physical; Electrochemistry; Energy & Fuels; Materials
Science, Multidisciplinary
SC Chemistry; Electrochemistry; Energy & Fuels; Materials Science
GA DY1KB
UT WOS:000384852800037
ER
PT J
AU Gilbert, AJ
McDonald, BS
Deinert, MR
AF Gilbert, Andrew J.
McDonald, Benjamin S.
Deinert, Mark R.
TI Advanced algorithms for radiographic material discrimination and
inspection system design
SO NUCLEAR INSTRUMENTS & METHODS IN PHYSICS RESEARCH SECTION B-BEAM
INTERACTIONS WITH MATERIALS AND ATOMS
LA English
DT Article
DE X-ray radiography; Neutron radiography; Dual-mode radiography; Material
discrimination; Special nuclear materials
ID FAST-NEUTRON RADIOGRAPHY; EXPLOSIVES DETECTION; CONTRABAND
AB X-ray and neutron radiography are powerful tools for non-invasively inspecting the interior of objects. However, current methods are limited in their ability to differentiate materials when multiple materials are present, especially within large and complex objects. Past work has demonstrated that the spectral shift that X-ray beams undergo in traversing an object can be used to detect and quantify nuclear materials. The technique uses a spectrally sensitive detector and an inverse algorithm that varies the composition of the object until the X-ray spectrum predicted by X-ray transport matches the one measured. Here we show that this approach can be adapted to multi-mode radiography, with energy integrating detectors, and that the Cramer-Rao lower bound can be used to choose an optimal set of inspection modes a priori. We consider multi-endpoint X-ray radiography alone, or in combination with neutron radiography using deuterium-deuterium (DD) or deuterium-tritium (DT) sources. We show that for an optimal mode choice, the algorithm can improve discrimination between high-Z materials, specifically between tungsten and plutonium, and estimate plutonium mass within a simulated nuclear material storage system to within 1%. (C) 2016 Elsevier B.V. All rights reserved.
C1 [Gilbert, Andrew J.; McDonald, Benjamin S.] Pacific Northwest Natl Lab, Richland, WA 99354 USA.
[Deinert, Mark R.] Colorado Sch Mines, Golden, CO 80401 USA.
RP McDonald, BS (reprint author), Pacific Northwest Natl Lab, Richland, WA 99354 USA.; Deinert, MR (reprint author), Colorado Sch Mines, Golden, CO 80401 USA.
EM benjamin.mcdonald@pnnl.gov; mdeinert@mines.edu
FU Office of Nonproliferation Research and Development, National Nuclear
Security Administration; Next Generation Safeguards Initiative, Office
of Nonproliferation and Arms Control; U.S. Department of Energy
[DE-AC05-76RL01830, PNNL-SA-113690]
FX This research was sponsored by the Office of Nonproliferation Research
and Development, National Nuclear Security Administration. A. J. Gilbert
was supported by the Next Generation Safeguards Initiative, Office of
Nonproliferation and Arms Control. A portion of the research was
performed using PNNL Institutional Computing at Pacific Northwest
National Laboratory. Pacific Northwest National Laboratory is operated
for the U.S. Department of Energy by Battelle under Contract
DE-AC05-76RL01830. PNNL-SA-113690.
NR 26
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U1 4
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PI AMSTERDAM
PA PO BOX 211, 1000 AE AMSTERDAM, NETHERLANDS
SN 0168-583X
EI 1872-9584
J9 NUCL INSTRUM METH B
JI Nucl. Instrum. Methods Phys. Res. Sect. B-Beam Interact. Mater. Atoms
PD OCT 15
PY 2016
VL 385
BP 51
EP 58
DI 10.1016/j.nimb.2016.07.013
PG 8
WC Instruments & Instrumentation; Nuclear Science & Technology; Physics,
Atomic, Molecular & Chemical; Physics, Nuclear
SC Instruments & Instrumentation; Nuclear Science & Technology; Physics
GA DY1RO
UT WOS:000384872300008
ER
PT J
AU Lieberman, HR
Farina, EK
Caldwell, J
Williams, KW
Thompson, LA
Niro, PJ
Grohmann, KA
McClung, JP
AF Lieberman, Harris R.
Farina, Emily K.
Caldwell, John
Williams, Kelly W.
Thompson, Lauren A.
Niro, Philip J.
Grohmann, Kyle A.
McClung, James P.
TI Cognitive function, stress hormones, heart rate and nutritional status
during simulated captivity in military survival training
SO PHYSIOLOGY & BEHAVIOR
LA English
DT Article
DE SERE school; Mood; Psychomotor vigilance (PVT); N-back task; Fatigue
ID PSYCHOLOGICAL STRESS; SALIVARY CORTISOL; SUSTAINED OPERATIONS;
TRANSFERRIN RECEPTOR; SLEEP-DEPRIVATION; PHYSICAL-ACTIVITY;
BODY-COMPOSITION; ADRENAL-FUNCTION; DECISION-MAKING; NEUROPEPTIDE-Y
AB Stress influences numerous psychological and physiological processes, and its effects have practical implications in a variety of professions and real-world activities. However, few studies have concurrently assessed multiple behavioral, hormonal, nutritional and heart-rate responses of humans to acute, severe stress. This investigation simultaneously assessed cognitive, affective, hormonal, and heart -rate responses induced by an intensely stressful real-world-environment designed to simulate wartime captivity. Sixty males were evaluated during and immediately following participation in U.S. Army Survival, Evasion, Resistance, and Escape (SERE) school, three weeks of intense but standardized training for Soldiers at risk of capture. Simulated captivity and intense mock interrogations degraded grammatical reasoning (p < 0.005), sustained-attention (p < 0.001), working memory (p <0.05) and all aspects of mood assessed by the Profile of Mood States (POMS) questionnaire: Tension/Anxiety, Depression/Dejection, Anger/Hostility, Vigor/Activity, Fatigue/Inertia; Confusion/Bewilderment, and Total Mood Disturbance (p < 0.001) It also elevated heart rate (p < 0.001); increased serum and salivary cortisol and dehydroepiandrosterone-sulfate (DHEA-s) (p < 0.01); elevated serum epinephrine, norepinephrine, and soluble transferrin receptors (sTfR) (p < 0.01); increased salivary neuropeptide-Y (NPY) (p < 0.001); and decreased serum prolactin and serum and salivary testosterone (p < 0.001). Partial recovery was observed immediately after training, but stress -induced changes, particularly in body weight and several of the biomarkers, persisted. This study demonstrates that when individuals were exposed to realistic and controlled simulated captivity, cognition, mood, stress hormones, nutritional status and heart rate are simultaneously altered, and each of these subsequently recovers at different rates. Published by Elsevier Inc.
C1 [Lieberman, Harris R.; Farina, Emily K.; Caldwell, John; Williams, Kelly W.; Thompson, Lauren A.; Niro, Philip J.; McClung, James P.] US Army Res Inst Environm Med, Mil Nutr Div, Gen Greene Ave,Bldg 42, Natick, MA 01760 USA.
[Farina, Emily K.; Caldwell, John; Williams, Kelly W.; Thompson, Lauren A.] Oak Ridge Inst Sci & Educ, Bekamp, MD 21017 USA.
[Grohmann, Kyle A.] USASOC, John F Kennedy Special Warfare Ctr & Sch, Ft Bragg, NC 28310 USA.
RP Lieberman, HR (reprint author), US Army Res Inst Environm Med, Mil Nutr Div, Gen Greene Ave,Bldg 42, Natick, MA 01760 USA.
EM harris.r.lieberman.civ@mail.mil
FU U.S. Army Medical Research and Materiel Command (USAMRMC)
FX This work was supported by core funding from the U.S. Army Medical
Research and Materiel Command (USAMRMC). The views, opinions, and
findings in this report are those of the authors and should not be
construed as an official Department of Defense or Army position, policy,
or decision, unless so designated by other official documentation.
Citations of commercial organizations and trade names in this report do
not constitute an official Department of the Army endorsement or
approval of the products or services of these organizations. The
investigators have adhered to the policies for protection of human
subjects as prescribed in DOD Instruction 3216.02 and the research was
conducted in adherence with the provisions of 32 CFR Part 219.
NR 89
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PI OXFORD
PA THE BOULEVARD, LANGFORD LANE, KIDLINGTON, OXFORD OX5 1GB, ENGLAND
SN 0031-9384
J9 PHYSIOL BEHAV
JI Physiol. Behav.
PD OCT 15
PY 2016
VL 165
BP 86
EP 97
DI 10.1016/j.physbeh.2016.06.037
PG 12
WC Psychology, Biological; Behavioral Sciences
SC Psychology; Behavioral Sciences
GA DY0LS
UT WOS:000384788900011
PM 27374427
ER
PT J
AU Jamison, RD
Shen, YL
AF Jamison, Ryan D.
Shen, Yu-Lin
TI Delamination analysis of metal-ceramic multilayer coatings subject to
nanoindentation
SO SURFACE & COATINGS TECHNOLOGY
LA English
DT Article; Proceedings Paper
CT 4th Biennial TACT International Thin Films Conference (TACT)
CY NOV 15-18, 2015
CL Natl Cheng Kung Univ, Tainan, TAIWAN
HO Natl Cheng Kung Univ
DE Nanoindentation; Multilayer coating; Delamination; Finite element
analysis
ID INDENTATION BEHAVIOR; MECHANICAL-BEHAVIOR; ELASTIC-MODULUS; THIN-FILMS;
COMPOSITES; PLASTICITY; HARDNESS; FAILURE; WEAR
AB Internal damage has been experimentally observed in aluminum (Al)/silicon carbide (SiC) multilayer coatings subject to nanoindentation loading. Post-indentation characterization has identified that delamination at the coating/substrate interface is the most prominent form of damage. In this study the finite element method is employed to study the effect of delamination on indentation-derived hardness and Young's modulus. The model features alternating Al/SiC nanolayers above a silicon (Si) substrate, in consistence with the actual material system used in earlier experiments. Cohesive elements with a traction separation relationship are used to facilitate delamination along the coating/substrate interface. Delamination is observed numerically to be sensitive to the critical normal and shear stresses that define the cohesive traction separation behavior. Axial tensile stress below the edge of indentation contact is found to be the largest contributor to damage initiation and evolution. Delamination results in a decrease in both indentation-derived hardness and Young's modulus. A unique finding is that delamination can occur during the unloading process of indentation, depending on the loading condition and critical tractions. (C) 2016 Elsevier B.V. All rights reserved.
C1 [Jamison, Ryan D.; Shen, Yu-Lin] Univ New Mexico, Dept Mech Engn, Albuquerque, NM 87131 USA.
[Jamison, Ryan D.] Sandia Natl Labs, Component Sci & Mech, POB 5800, Albuquerque, NM 87185 USA.
RP Shen, YL (reprint author), Univ New Mexico, Dept Mech Engn, Albuquerque, NM 87131 USA.
EM shenyl@unm.edu
NR 32
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U1 10
U2 10
PU ELSEVIER SCIENCE SA
PI LAUSANNE
PA PO BOX 564, 1001 LAUSANNE, SWITZERLAND
SN 0257-8972
J9 SURF COAT TECH
JI Surf. Coat. Technol.
PD OCT 15
PY 2016
VL 303
BP 3
EP 11
DI 10.1016/j.surfcoat.2016.01.038
PN A
PG 9
WC Materials Science, Coatings & Films; Physics, Applied
SC Materials Science; Physics
GA DY1LU
UT WOS:000384857300002
ER
PT J
AU Zhou, HB
Wang, JL
Jiang, W
Lu, GH
Aguiar, JA
Liu, F
AF Zhou, Hong-Bo
Wang, Jin-Long
Jiang, W.
Lu, Guang-Hong
Aguiar, J. A.
Liu, Feng
TI Electrophobic interaction induced impurity clustering in metals
SO ACTA MATERIALIA
LA English
DT Article
DE Electrophobic interaction; Impurity clustering; Metals
ID XENON BUBBLES; LOW-ENERGY; TUNGSTEN; ALUMINUM; HYDROGEN; IRRADIATION;
MOLYBDENUM; RETENTION; DIFFUSION; SURFACES
AB We introduce the concept of electrophobic interaction, analogous to hydrophobic interaction, for describing the behavior of impurity atoms in a metal, a "solvent of electrons". We demonstrate that there exists a form of electrophobic interaction between impurities with closed electron shell structure, which governs their dissolution behavior in a metal. Using He, Be and Ar as examples, we predict by first principles calculations that the electrophobic interaction drives He, Be or Ar to form a close-packed cluster with a clustering energy that follows a universal power-law scaling with the number of atoms (N) dissolved in a free electron gas, as well as W or Al lattice, as E-c proportional to (N-2/3-N). This new concept unifies the explanation for a series of experimental observations of close-packed inert-gas bubble formation in metals, and significantly advances our fundamental understanding and capacity to predict the solute behavior of impurities in metals, a useful contribution to be considered in future material design of metals for nuclear, metallurgical, and energy applications. (C) 2016 Acta Materialia Inc. Published by Elsevier Ltd. All rights reserved.
C1 [Zhou, Hong-Bo; Wang, Jin-Long; Lu, Guang-Hong] Beihang Univ, Dept Phys, Beijing 100191, Peoples R China.
[Zhou, Hong-Bo; Wang, Jin-Long; Lu, Guang-Hong] Beihang Univ, Beijing Key Lab Adv Nucl Mat & Phys, Beijing 100191, Peoples R China.
[Jiang, W.; Liu, Feng] Univ Utah, Dept Mat Sci & Engn, Salt Lake City, UT 84112 USA.
[Aguiar, J. A.] Natl Renewable Energy Lab, Golden, CO USA.
[Aguiar, J. A.] Los Alamos Natl Lab, POB 1663, Los Alamos, NM 87545 USA.
[Liu, Feng] Collaborat Innovat Ctr Quantum Matter, Beijing 100084, Peoples R China.
RP Lu, GH (reprint author), Beihang Univ, Dept Phys, Beijing 100191, Peoples R China.; Liu, F (reprint author), Univ Utah, Dept Mat Sci & Engn, Salt Lake City, UT 84112 USA.; Aguiar, JA (reprint author), Natl Renewable Energy Lab, Golden, CO USA.
EM Igh@buaa.edu.cn; jeffery.aguiar@nrel.gov; fliu@eng.utah.edu
OI Aguiar, Jeffery/0000-0001-6101-4762
FU National Magnetic Confinement Fusion Program [2013GB109002]; National
Natural Science Foundation of China [11405006, 51325103]; China
Scholarship Council [201506025054]; Oak Ridge National Laboratory's
Center User Facility; Scientific User Facilities Division, Office of
Basic Energy Sciences, U.S. Department of Energy; DOE-BES
[DE-FG02-04ER46148]
FX This research is supported by the National Magnetic Confinement Fusion
Program with Grant No. 2013GB109002, the National Natural Science
Foundation of China with Grant No. 11405006, and the China Scholarship
Council with Grant No. 201506025054. G.H. Lu acknowledges the financial
support from the National Natural Science Foundation of China for
Distinguished Young Scientists through Grant No. 51325103. J.A. Aguiar
acknowledges support in part by Oak Ridge National Laboratory's Center
User Facility, which is sponsored by the Scientific User Facilities
Division, Office of Basic Energy Sciences, U.S. Department of Energy. F.
Liu acknowledges the financial support from DOE-BES (No.
DE-FG02-04ER46148).
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PU PERGAMON-ELSEVIER SCIENCE LTD
PI OXFORD
PA THE BOULEVARD, LANGFORD LANE, KIDLINGTON, OXFORD OX5 1GB, ENGLAND
SN 1359-6454
EI 1873-2453
J9 ACTA MATER
JI Acta Mater.
PD OCT 15
PY 2016
VL 119
BP 1
EP 8
DI 10.1016/j.actamat.2016.08.005
PG 8
WC Materials Science, Multidisciplinary; Metallurgy & Metallurgical
Engineering
SC Materials Science; Metallurgy & Metallurgical Engineering
GA DY0HQ
UT WOS:000384778300001
ER
PT J
AU Ozawa, R
Hayami, S
Barros, K
Chern, GW
Motome, Y
Batista, CD
AF Ozawa, Ryo
Hayami, Satoru
Barros, Kipton
Chern, Gia-Wei
Motome, Yukitoshi
Batista, Cristian D.
TI Vortex Crystals with Chiral Stripes in Itinerant Magnets
SO JOURNAL OF THE PHYSICAL SOCIETY OF JAPAN
LA English
DT Article
ID BERRY PHASE; LATTICE; FERROMAGNET
AB We study noncoplanar magnetic ordering in frustrated itinerant magnets. For a family of Kondo square lattice models with classical local moments, we find that a double-Q noncoplanar vortex crystal has lower energy than the single-Q helical order expected from the Ruderman-Kittel-Kasuya-Yosida interaction when the lattice symmetry dictates four global maxima in the bare magnetic susceptibility. By expanding in the small Kondo exchange and the degree of noncoplanarity, we demonstrate that this noncoplanar state arises from a Fermi surface instability occurring in independent sections connected by two ordering wave vectors.
C1 [Ozawa, Ryo; Motome, Yukitoshi] Univ Tokyo, Dept Appl Phys, Bunkyo Ku, Tokyo 1138656, Japan.
[Hayami, Satoru] Hokkaido Univ, Dept Phys, Sapporo, Hokkaido 0600810, Japan.
[Barros, Kipton] Los Alamos Natl Lab, Theoret Div, Los Alamos, NM 87545 USA.
[Barros, Kipton] Los Alamos Natl Lab, CNLS, Los Alamos, NM 87545 USA.
[Chern, Gia-Wei] Univ Virginia, Dept Phys, Charlottesville, VA 22904 USA.
[Batista, Cristian D.] Univ Tennessee, Dept Phys & Astron, Knoxville, TN 37996 USA.
[Batista, Cristian D.] Oak Ridge Natl Lab, Quantum Condensed Matter Div, Oak Ridge, TN 37831 USA.
[Batista, Cristian D.] Oak Ridge Natl Lab, Shull Wollan Ctr, Oak Ridge, TN 37831 USA.
RP Ozawa, R (reprint author), Univ Tokyo, Dept Appl Phys, Bunkyo Ku, Tokyo 1138656, Japan.
EM ozawa@aion.t.u-tokyo.ac.jp
OI Barros, Kipton/0000-0002-1333-5972
FU Japan Society for the Promotion of Science; Program for Leading Graduate
Schools (ALPS); Strategic Programs for Innovative Research (SPIRE),
MEXT; Computational Materials Science Initiative (CMSI), Japan; U.S. DOE
through LDRD program [DE-AC52-06NA25396]; [24340076]
FX We thank S. Blugel, Y. Kato, S. Kumar, S.-Z. Lin, T. Misawa, M. Udagawa,
A. Uehara, Y. Yamaji, and T. Ziman for fruitful discussions. The KPM-LD
simulations were carried out at the Supercomputer Center, Institute for
Solid State Physics, University of Tokyo. R.O. was supported by the
Japan Society for the Promotion of Science through a research fellowship
for young scientists and the Program for Leading Graduate Schools
(ALPS). R.O. also acknowledges the CNLS summer student program at LANL.
This research was supported by Grants-in-Aid for Scientific Research
(No. 24340076), the Strategic Programs for Innovative Research (SPIRE),
MEXT, and the Computational Materials Science Initiative (CMSI), Japan.
Work at LANL was carried out under the auspices of U.S. DOE contract No.
DE-AC52-06NA25396 through the LDRD program.
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PU PHYSICAL SOC JAPAN
PI TOKYO
PA YUSHIMA URBAN BUILDING 5F, 2-31-22 YUSHIMA, BUNKYO-KU, TOKYO, 113-0034,
JAPAN
SN 0031-9015
J9 J PHYS SOC JPN
JI J. Phys. Soc. Jpn.
PD OCT 15
PY 2016
VL 85
IS 10
AR 103703
DI 10.7566/JPSJ.85.103703
PG 5
WC Physics, Multidisciplinary
SC Physics
GA DX3ON
UT WOS:000384282500001
ER
PT J
AU Kacher, J
Hattar, K
Robertson, IM
AF Kacher, Josh
Hattar, Khalid
Robertson, Ian M.
TI Initial texture effects on the thermal stability and grain growth
behavior of nanocrystalline Ni thin films
SO MATERIALS SCIENCE AND ENGINEERING A-STRUCTURAL MATERIALS PROPERTIES
MICROSTRUCTURE AND PROCESSING
LA English
DT Article
DE Abnormal grain growth; Nanocrystalline; In situ transmission electron
microscopy; Transmission Kikuchi diffraction; EBSD
ID TRANSMISSION KIKUCHI DIFFRACTION; SCANNING-ELECTRON-MICROSCOPE; LASER
DEPOSITED NICKEL; BOUNDARY MIGRATION; SURFACE-ENERGY; METALS; ALLOYS;
STAGNATION; SIMULATION; EVOLUTION
AB Nanocrystalline Ni thin films with different as-deposited textures were synthesized by varying the substrate temperature during pulsed-laser deposition. The influence of initial texture variations on the thermal stability and annealing behavior of the thin films was studied via in situ transmission electron microscopy annealing and transmission Kikuchi diffraction analysis. It was found that, as the substrate temperature during deposition was increased, the initial microstructure varied from a random distribution of grains to one almost entirely composed of (001) oriented grains, with the volume fraction of (001) oriented grains increasing with increasing substrate temperature. The (001) oriented grains increased thermal stability and constrained grain growth during annealing, resulting in a bimodal grain size distribution in the annealed films. Despite different surface orientations after annealing, the misorientation distribution functions for the films were similar, suggesting that the boundary state is a primary factor in dictating equilibrium. (C) 2016 Elsevier B.V. All rights reserved.
C1 [Kacher, Josh] Georgia Inst Technol, Atlanta, GA 30332 USA.
[Hattar, Khalid] Sandia Natl Labs, POB 5800, Albuquerque, NM 87185 USA.
[Robertson, Ian M.] Univ Wisconsin, Madison, WI 53706 USA.
RP Kacher, J (reprint author), Georgia Inst Technol, Atlanta, GA 30332 USA.
EM josh.kacher@mse.gatech.edu
FU US Department of Energy Office of Basic Energy Sciences, Division of
Materials Science [DEFG-02-07ER46443]; U.S. Department of Energy's
National Nuclear Security Administration [DE-AC04-94AL85000]; Division
of Materials Science and Engineering, Office of Basic Energy Sciences,
U.S. Department of Energy at Sandia
FX The authors would like to thanks R. Goeke and B.G. Clark for useful
discussion. JK and IMR acknowledge support by the US Department of
Energy Office of Basic Energy Sciences, Division of Materials Science,
under Award no. DEFG-02-07ER46443. TKD characterization was done at
EDAX-TSL facilities in Draper, Utah. Sandia National Laboratories is a
multi-program laboratory operated by Sandia Corporation, a wholly owned
subsidiary of Lock-heed Martin company, for the U.S. Department of
Energy's National Nuclear Security Administration under contract
DE-AC04-94AL85000. KH acknowledges support from the Division of
Materials Science and Engineering, Office of Basic Energy Sciences, U.S.
Department of Energy at Sandia.
NR 60
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U1 15
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PU ELSEVIER SCIENCE SA
PI LAUSANNE
PA PO BOX 564, 1001 LAUSANNE, SWITZERLAND
SN 0921-5093
EI 1873-4936
J9 MAT SCI ENG A-STRUCT
JI Mater. Sci. Eng. A-Struct. Mater. Prop. Microstruct. Process.
PD OCT 15
PY 2016
VL 675
BP 110
EP 119
DI 10.1016/j.msea.2016.08.045
PG 10
WC Nanoscience & Nanotechnology; Materials Science, Multidisciplinary;
Metallurgy & Metallurgical Engineering
SC Science & Technology - Other Topics; Materials Science; Metallurgy &
Metallurgical Engineering
GA DX4XF
UT WOS:000384383700012
ER
PT J
AU Miller, VM
Berman, TD
Beyerlein, IJ
Jones, JW
Pollock, TM
AF Miller, Victoria M.
Berman, Tracy D.
Beyerlein, Irene J.
Jones, J. Wayne
Pollock, Tresa M.
TI Prediction of the plastic anisotropy of magnesium alloys with synthetic
textures and implications for the effect of texture on formability
SO MATERIALS SCIENCE AND ENGINEERING A-STRUCTURAL MATERIALS PROPERTIES
MICROSTRUCTURE AND PROCESSING
LA English
DT Article
DE Magnesium alloys; Viscoplastic self-consistent model; Formability;
Texture
ID ENHANCED STRETCH FORMABILITY; CHANNEL ANGULAR EXTRUSION; RARE EARTH
ALLOYS; GRAIN-SIZE; MG ALLOY; DEFORMATION-BEHAVIOR; ROOM-TEMPERATURE;
PRISMATIC SLIP; MECHANICAL-PROPERTIES; NEUTRON-DIFFRACTION
AB Crystallographic texture is a well-known microstructural feature influencing the formability of magnesium alloys. However, the effects of individual texture characteristics common after thermomechanical processing have not been isolated due to the experimental challenge associated with varying them independently. Similarly, the effect of the propensity for twinning on formability, which both accommodates deformation and reorients the crystal, have not been systematically studied. This study uses synthetic sheet textures in conjunction with a viscoplastic self-consistent (VPSC) polycrystal plasticity model to predict deformation and formability behavior. The VPSC model was first parameterized based on experimental mechanical data and textures from fine-grained thixomolded and thermomechanically processed AZ61L. Subsequently, synthetic textures were generated to examine the effects of basal peak intensity, prismatic plane distribution, and asymmetry of the basal pole figure peak. Of these texture characteristics, basal peak strength is the most important predictor of forming behavior, with prismatic plane distribution and c-axis anisotropy resulting in comparatively weak effects. In the second part of the study, the effective critical resolved shear stress for twinning was varied, resulting in poorer forming behavior with easier twin activation. In both cases, increasing prismatic slip activity was deleterious to the predicted forming behavior. (C) 2016 Elsevier B.V. All rights reserved.
C1 [Miller, Victoria M.; Pollock, Tresa M.] Univ Calif Santa Barbara, Dept Mat, Santa Barbara, CA 93106 USA.
[Berman, Tracy D.; Jones, J. Wayne] Dept Mat Sci & Engn, 2300 Hayward St, Ann Arbor, MI 48109 USA.
[Beyerlein, Irene J.] Los Alamos Natl Lab, Div Theoret, Los Alamos, NM 87545 USA.
RP Miller, VM (reprint author), Univ Calif Santa Barbara, Dept Mat, Santa Barbara, CA 93106 USA.
EM vmiller@umail.ucsb.edu
FU University of California Santa Barbara; Office of Naval Research
[N00014-12-1-0399]; Laboratory Directed Research and Development program
[20140348ER]
FX The authors would like to express their gratitude to Ray Decker and
nanoMAG, LLC for providing the material used in this study. V. M. Miller
additionally thanks the University of California Santa Barbara for the
support of a Regents' Special Fellowship and T.M. Pollock acknowledges
the support of Office of Naval Research Grant number N00014-12-1-0399.
I.J. Beyerlein gratefully acknowledges support by a Laboratory Directed
Research and Development program 20140348ER.
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PU ELSEVIER SCIENCE SA
PI LAUSANNE
PA PO BOX 564, 1001 LAUSANNE, SWITZERLAND
SN 0921-5093
EI 1873-4936
J9 MAT SCI ENG A-STRUCT
JI Mater. Sci. Eng. A-Struct. Mater. Prop. Microstruct. Process.
PD OCT 15
PY 2016
VL 675
BP 345
EP 360
DI 10.1016/j.msea.2016.08.063
PG 16
WC Nanoscience & Nanotechnology; Materials Science, Multidisciplinary;
Metallurgy & Metallurgical Engineering
SC Science & Technology - Other Topics; Materials Science; Metallurgy &
Metallurgical Engineering
GA DX4XF
UT WOS:000384383700036
ER
PT J
AU Alam, ME
Pal, S
Fields, K
Maloy, SA
Hoelzer, DT
Odette, GR
AF Alam, M. E.
Pal, S.
Fields, K.
Maloy, S. A.
Hoelzer, D. T.
Odette, G. R.
TI Tensile deformation and fracture properties of a 14YWT nanostructured
ferritic alloy
SO MATERIALS SCIENCE AND ENGINEERING A-STRUCTURAL MATERIALS PROPERTIES
MICROSTRUCTURE AND PROCESSING
LA English
DT Article
DE Nanostructured ferritic alloy; Nano oxide; Delamination; Tensile
properties; Fractography
ID STRENGTHENING MECHANISMS; TEMPERATURE-DEPENDENCE; TOUGHNESS PROPERTIES;
STEELS; 13CR-1W-0.3TI-0.3Y(2)O(3); MICROSTRUCTURE
AB A new larger heat of a 14YWT nanostructured ferritic alloy (NFA), FCRD NFA-1, was synthesized by ball milling FeO and argon atomized Fe-14Cr-3W-0.4Ti-0.2Y (wt%) powders, followed by hot extrusion, annealing and cross rolling to produce an approximate to 10 mm-thick plate. NFA-1 contains a bimodal size distribution of pancake-shaped, mostly very fine scale, grains. The as-processed plate also contains a large population of microcracks running parallel to its broad surfaces. The small grains and large concentration of Y-Ti-O nano-oxides (NOs) result in high strength up to 800 degrees C. The uniform and total elongations range from approximate to 1-8%, and approximate to 10-24%, respectively. The strength decreases more rapidly above approximate to 400 degrees C and deformation transitions to largely viscoplastic creep by P.approximate to 600 degrees C. While the local fracture mechanism is generally ductile-dimple microvoid nucleation, growth and coalescence, perhaps the most notable feature of tensile deformation behavior of NFA-1 is the occurrence of periodic delamination, manifested as fissures on the fracture surfaces. (C) 2016 Elsevier B.V. All rights reserved.
C1 [Alam, M. E.; Pal, S.; Fields, K.; Odette, G. R.] Univ Calif Santa Barbara, Dept Mat, Santa Barbara, CA 93106 USA.
[Maloy, S. A.] Los Alamos Natl Lab, Los Alamos, NM 87545 USA.
[Hoelzer, D. T.] Oak Ridge Natl Lab, Div Mat Sci & Technol, Oak Ridge, TN 37830 USA.
RP Alam, ME (reprint author), Univ Calif Santa Barbara, Dept Mat, Santa Barbara, CA 93106 USA.
EM alam@engineering.ucsb.edu
OI Maloy, Stuart/0000-0001-8037-1319
FU U.S. Department of Energy Office of Fusion Energy Sciences
[DE-FG03-94ER54275]; Office of Nuclear Energy university programs
[00119430 8-442520-59048]
FX The authors gratefully acknowledge the support received for this
research work by the U.S. Department of Energy Office of Fusion Energy
Sciences (DE-FG03-94ER54275) and the Office of Nuclear Energy university
programs administered by INL (IDNL Award #00119430 8-442520-59048).
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PU ELSEVIER SCIENCE SA
PI LAUSANNE
PA PO BOX 564, 1001 LAUSANNE, SWITZERLAND
SN 0921-5093
EI 1873-4936
J9 MAT SCI ENG A-STRUCT
JI Mater. Sci. Eng. A-Struct. Mater. Prop. Microstruct. Process.
PD OCT 15
PY 2016
VL 675
BP 437
EP 448
DI 10.1016/j.msea.2016.08.051
PG 12
WC Nanoscience & Nanotechnology; Materials Science, Multidisciplinary;
Metallurgy & Metallurgical Engineering
SC Science & Technology - Other Topics; Materials Science; Metallurgy &
Metallurgical Engineering
GA DX4XF
UT WOS:000384383700046
ER
PT J
AU Delaire, C
van Genuchten, CM
Amrose, SE
Gadgil, AJ
AF Delaire, Caroline
van Genuchten, Case M.
Amrose, Susan E.
Gadgil, Ashok J.
TI Bacteria attenuation by iron electrocoagulation governed by interactions
between bacterial phosphate groups and Fe(III) precipitates
SO WATER RESEARCH
LA English
DT Article
DE Iron electrocoagulation; Bacteria attenuation; Bacterial surface
functional groups; Specific interactions; Bivalent cations; Oxyanions
ID FECAL INDICATOR BACTERIA; NATURAL ORGANIC-MATTER; ATR-FTIR SPECTROSCOPY;
ESCHERICHIA-COLI; HYDROGEN-PEROXIDE; METAL ADSORPTION; ARSENIC REMOVAL;
WATER; ADHESION; SURFACE
AB Iron electrocoagulation (Fe-EC) is a low-cost process in which Fe(II) generated from an Fe(0) anode reacts with dissolved O-2 to form (1) Fe(III) precipitates with an affinity for bacterial cell walls and (2) bactericidal reactive oxidants. Previous work suggests that Fe-EC is a promising treatment option for groundwater containing arsenic and bacterial contamination. However, the mechanisms of bacteria attenuation and the impact of major groundwater ions are not well understood. In this work, using the model indicator Escherichia coli (E. coli), we show that physical removal via enmeshment in EC precipitate flocs is the primary process of bacteria attenuation in the presence of HCO3-, which significantly inhibits inactivation, possibly due to a reduction in the lifetime of reactive oxidants. We demonstrate that the adhesion of EC precipitates to cell walls, which results in bacteria encapsulation in flocs, is driven primarily by interactions between EC precipitates and phosphate functional groups on bacteria surfaces. In single solute electrolytes, both P (0.4 mM) and Ca/Mg (1-13 mM) inhibited the adhesion of EC precipitates to bacterial cell walls, whereas Si (0.4 mM) and ionic strength (2-200 mM) did not impact E. coli attenuation. Interestingly, P (0.4 mM) did not affect E. coli attenuation in electrolytes containing Ca/Mg, consistent with bivalent cation bridging between bacterial phosphate groups and inorganic P sorbed to EC precipitates. Finally, we found that EC precipitate adhesion is largely independent of cell wall composition, consistent with comparable densities of phosphate functional groups on Gram-positive and Gram-negative cells. Our results are critical to predict the performance of Fe-EC to eliminate bacterial contaminants from waters with diverse chemical compositions. (C) 2016 Elsevier Ltd. All rights reserved.
C1 [Delaire, Caroline; Amrose, Susan E.; Gadgil, Ashok J.] Univ Calif Berkeley, Dept Civil & Environm Engn, Berkeley, CA 94720 USA.
[van Genuchten, Case M.] Univ Utrecht, Fac Geosci, Dept Earth Sci Geochem, NL-3508 TA Utrecht, Netherlands.
[Gadgil, Ashok J.] Lawrence Berkeley Natl Lab, Energy Technol Area, Berkeley, CA 94720 USA.
RP Delaire, C (reprint author), Univ Calif Berkeley, Dept Civil & Environm Engn, Berkeley, CA 94720 USA.
EM caroline.delaire@orange.fr
FU Development Impact Lab (USAID) of the USAID Higher Education Solutions
Network [AID-OAA-A-13-00002]; Andrew and Virginia Rudd Family Foundation
Chair for Safe Water and Sanitation; Netherlands Organization for
Scientific Research (NWO) through a Veni grant [14400]; Office of
Science, Office of Basic Energy Sciences of the U.S. Department of
Energy [DE-AC02-05CH11231]
FX This work was supported by the Development Impact Lab (USAID Cooperative
Agreement AID-OAA-A-13-00002), part of the USAID Higher Education
Solutions Network, and the Andrew and Virginia Rudd Family Foundation
Chair for Safe Water and Sanitation administered by the Blum Center for
Developing Economies. Additionally, C.M.v.G. acknowledges funding
support from the Netherlands Organization for Scientific Research (NWO)
through a Veni grant (proposal #14400). We wish to express our gratitude
to Kara Nelson, who provided useful discussions regarding the
complexation of Ca/Mg to bacterial functional groups, and to David
Sedlak, Denise Schichnes, John Wertz, and Aidan Cecchetti for their kind
assistance along various steps of this work. zeta-potential measurements
were conducted at the Molecular Foundry of Lawrence Berkeley National
Laboratory and supported by the Office of Science, Office of Basic
Energy Sciences, of the U.S. Department of Energy under Contract No.
DE-AC02-05CH11231.
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PI OXFORD
PA THE BOULEVARD, LANGFORD LANE, KIDLINGTON, OXFORD OX5 1GB, ENGLAND
SN 0043-1354
J9 WATER RES
JI Water Res.
PD OCT 15
PY 2016
VL 103
BP 74
EP 82
DI 10.1016/j.watres.2016.07.020
PG 9
WC Engineering, Environmental; Environmental Sciences; Water Resources
SC Engineering; Environmental Sciences & Ecology; Water Resources
GA DV9WE
UT WOS:000383292100009
PM 27438902
ER
PT J
AU Zou, YQ
Yang, CB
Wu, DS
Yan, C
Zeng, MS
Lan, YY
Dai, ZX
AF Zou, Youqin
Yang, Changbing
Wu, Daishe
Yan, Chun
Zeng, Masun
Lan, Yingying
Dai, Zhenxue
TI Probabilistic assessment of shale gas production and water demand at
Xiuwu Basin in China
SO APPLIED ENERGY
LA English
DT Article
DE Shale gas; Probabilistic analysis; Monte Carlo simulation; Water
consumption; Sensitivity analysis
ID NATURAL-GAS; SENSITIVITY-ANALYSIS; ASIA-PACIFIC; IMPACTS; MODEL;
EMISSIONS; RESERVES; CHALLENGES; RESOURCES; ENERGY
AB This study presents an integrated probabilistic framework by combining Monte Carlo Simulation with a gas transport model of a horizontal well with multi-fracturing stages to assess shale gas resources in the Wangyinpu Formation of the Xiuwu Basin, China. Modeling results suggest that the 30-year cumulative production of a single horizontal well is predicted at a likely value of 3.50 x 10(8) m(3) with a maximum of 6.78 x 10(9) m3. Potential shale gas production from a "sweet spot" area is estimated at a range of 1.13 x 10(19)-1.76 x 10(13) m(3) with a likely value of 8.24 x 10(11) m(3). Sensitivity analysis indicates that the gas production rate and cumulative gas production of a single horizontal well are most sensitive to the relative volume occupied by kerogen in the bulk volume of the shale, gas desorption rate, number of fracturing stages, and permeability of the stimulated zone. Assessment of water demand for horizontal well drilling and hydraulic fracturing suggests that shale gas development at the Xiuwu Basin will not likely cause regional water-supply stress because of abundant water resources in the region. The probabilistic approach presented in this study can provide valuable information for planning shale gas development and can also be applied to other shale gas reservoirs. (C) 2016 Elsevier Ltd. All rights reserved.
C1 [Zou, Youqin; Wu, Daishe] Nanchang Univ, Sch Resources Environm & Chem Engn, Nanchang 330031, Jiangxi, Peoples R China.
[Zou, Youqin; Wu, Daishe] Nanchang Univ, Minist Educ, Key Lab Poyang Lake Ecol & Bioresource Utilizat, Nanchang 330047, Jiangxi, Peoples R China.
[Yang, Changbing] Univ Texas Austin, Bur Econ Geol, Austin, TX 78758 USA.
[Yan, Chun] Jiangxi Inst Geoenvironm Monitoring, Nanchang 330095, Jiangxi, Peoples R China.
[Zeng, Masun] Jiangxi Prov Invest Design & Res Inst, Nanchang 330095, Jiangxi, Peoples R China.
[Lan, Yingying] Nanchang Inst Technol, Nanchang 330099, Jiangxi, Peoples R China.
[Dai, Zhenxue] Los Alamos Natl Lab, Earth & Environm Sci Div, Los Alamos, NM 87545 USA.
RP Zou, YQ (reprint author), Nanchang Univ, Sch Resources Environm & Chem Engn, Nanchang 330031, Jiangxi, Peoples R China.; Yang, CB (reprint author), Univ Texas Austin, Bur Econ Geol, Austin, TX 78758 USA.
EM zouyouqin@ncu.edu.cn; changbing.yang@beg.utexas.edu
OI Dai, Zhenxue/0000-0002-0805-7621
FU Jiangxi province as a key project in Achievements in Science and
Technology through project of Assessment of Shale Gas Resources in
Jiangxi Province; Determination of Key Factors for Exploration
[20124ABE02104]; Chinese National Science Foundation through project of
Migration of hazardous elements [41173115]
FX This study has been funded by Jiangxi province as a key project in
Achievements in Science and Technology through the project of Assessment
of Shale Gas Resources in Jiangxi Province and Determination of Key
Factors for Exploration (Project #20124ABE02104) and by Chinese National
Science Foundation through the project of Migration of hazardous
elements caused by coal mining and potential impacts on environments
(Project #41173115). We also thank Stephanie Jones from Bureau of
Economic Geology, The University of Texas at Austin, who edited the
manuscript. The authors want to thank for the reviewers and Dr. Jinyue
Yan, the Chief-in-editor of Applied Energy for their constructive
comments and suggestions for greatly improving this manuscript.
NR 55
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PI OXFORD
PA THE BOULEVARD, LANGFORD LANE, KIDLINGTON, OXFORD OX5 1GB, OXON, ENGLAND
SN 0306-2619
EI 1872-9118
J9 APPL ENERG
JI Appl. Energy
PD OCT 15
PY 2016
VL 180
BP 185
EP 195
DI 10.1016/j.apenergy.2016.07.099
PG 11
WC Energy & Fuels; Engineering, Chemical
SC Energy & Fuels; Engineering
GA DV9WC
UT WOS:000383291900015
ER
PT J
AU Rapin, W
Meslin, PY
Maurice, S
Vaniman, D
Nachon, M
Mangold, N
Schroder, S
Gasnault, O
Forni, O
Wiens, RC
Martinez, GM
Cousin, A
Sautter, V
Lasue, J
Rampe, EB
Archer, D
AF Rapin, W.
Meslin, P. -Y.
Maurice, S.
Vaniman, D.
Nachon, M.
Mangold, N.
Schroder, S.
Gasnault, O.
Forni, O.
Wiens, R. C.
Martinez, G. M.
Cousin, A.
Sautter, V.
Lasue, J.
Rampe, E. B.
Archer, D.
TI Hydration state of calcium sulfates in Gale crater, Mars: Identification
of bassanite veins
SO EARTH AND PLANETARY SCIENCE LETTERS
LA English
DT Article
DE Mars; calcium sulfate; bassanite; LIBS; hydrogen; ChemCam
ID CHEMCAM INSTRUMENT SUITE; OMEGA/MARS EXPRESS; GYPSUM; ANHYDRITE;
STABILITY; SEDIMENTS; PHASE; BASIN; UNIT
AB In-situ analyses reveal the presence of hydrogen within calcium sulfate veins crosscutting the sediments found in Gale crater. Laboratory experiments were performed to calibrate the hydrogen signal measured by laser induced breakdown spectroscopy (LIBS) in a range applicable to martian data. The analyses indicate that all veins targeted so far at Gale consist predominantly of bassanite which most likely formed by dehydration of gypsum. This scenario suggests that the percolating water produced gypsum, possibly by hydration of anhydrite in aqueous solution, and remained at temperatures below 60 degrees C at that time. Desiccating conditions followed, consistent with a hyperarid climate and favored by burial or impacts. Additionally, anhydrite with lesser bassanite has been found by XRD in samples of sediments hosting the veins. Our result suggests bassanite is likely found in the veins and anhydrite may be more common as a fine-grained component within the sediments. (C) 2016 Elsevier B.V. All rights reserved.
C1 [Rapin, W.; Meslin, P. -Y.; Maurice, S.; Gasnault, O.; Forni, O.; Cousin, A.; Lasue, J.] Univ Toulouse, UPS OMP, Toulouse, France.
[Rapin, W.; Meslin, P. -Y.; Maurice, S.; Schroder, S.; Gasnault, O.; Forni, O.; Cousin, A.; Lasue, J.] CNRS, Inst Rech Astrophys & Planetol, UMR 5277, Toulouse, France.
[Vaniman, D.] Planetary Sci Inst, Tucson, AZ USA.
[Nachon, M.; Mangold, N.] Univ Nantes, CNRS, Lab Planetol & Geodynam Nantes, UMR6112, Nantes, France.
[Wiens, R. C.] Los Alamos Natl Lab, Los Alamos, NM USA.
[Martinez, G. M.] Univ Michigan, Ann Arbor, MI 48109 USA.
[Sautter, V.] Museum Natl Hist Nat, Lab Mineral & Cosmochim Museum, Paris, France.
[Rampe, E. B.] NASA Johnson Space Ctr, Aerodyne Ind, Houston, TX USA.
[Archer, D.] NASA Johnson Space Ctr, Houston, TX USA.
RP Rapin, W (reprint author), IRAP CNRS, 9 Ave Colonel Roche, F-31028 Toulouse, France.
EM william.rapin@irap.omp.eu
FU Universite Paul Sabatier, Institut de Recherche en Astrophysique et
Planetologie (IRAP); CNES; NASA Mars Exploration Program
FX This research was funded by Universite Paul Sabatier as part of a PhD
thesis, and experiments were conducted at Institut de Recherche en
Astrophysique et Planetologie (IRAP) with support from CNES. Funding for
MSL and ChemCam operations and science in the US were provided by the
NASA Mars Exploration Program. Funding for ChemCam operations in France
was provided by CNES. The authors gratefully acknowledge the support of
all of the people at JPL involved in making MSL a successful mission.
The Raman spectroscopy analysis to assess the purity of the calcium
sulfate pellets was performed by Olivier Beyssac and Sylvain Bernard
from the Institut de Mineralogie, de Physique des Materiaux et de
Cosmochimie (IMPMC). The authors thankfully recognize their valuable
help. The authors also thank Mikhail Zolotov and one anonymous reviewer
for their helpful comments.
NR 53
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U1 32
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PU ELSEVIER SCIENCE BV
PI AMSTERDAM
PA PO BOX 211, 1000 AE AMSTERDAM, NETHERLANDS
SN 0012-821X
EI 1385-013X
J9 EARTH PLANET SC LETT
JI Earth Planet. Sci. Lett.
PD OCT 15
PY 2016
VL 452
BP 197
EP 205
DI 10.1016/j.epsl.2016.07.045
PG 9
WC Geochemistry & Geophysics
SC Geochemistry & Geophysics
GA DV5YE
UT WOS:000383005800019
ER
PT J
AU Abbaslou, S
Gatdula, R
Lu, M
Stein, A
Soref, RA
Jiang, W
AF Abbaslou, Siamak
Gatdula, Robert
Lu, Ming
Stein, Aaron
Soref, Richard A.
Jiang, Wei
TI High-Spectral-Contrast Symmetric Modes in Photonic Crystal Dual Nanobeam
Resonators
SO IEEE PHOTONICS TECHNOLOGY LETTERS
LA English
DT Article
DE Photonic crystals; silicon photonics; wavelength filtering devices;
coupled resonators; all-optical devices; optical switching devices;
guided waves; integrated optics devices
ID CAVITIES; COMPACT; MODULATOR
AB We demonstrate accurate control of mode symmetry in suspended dual-nanobeam resonators on a silicon-on-insulator chip. Each nanobeam consists of a Fabry-Perot nanocavity bounded by tapered 1-D photonic crystals. Even and odd cavity-modes are formed due to lateral evanescent coupling between the two nanobeams. The odd cavity-mode can be excited by mode-symmetry-transforming Mach-Zehnder couplers. Modal contrasts over 27 dB are measured in fabricated structures. The influence of the optical field in the middle air slot on the background transmission and quality factors is discussed. The observed peak wavelength separations of the modes at various nanobeam spacings are in good agreement with simulation results. These nanobeam resonators are potentially useful in applications, such as ultrafast all-optical modulation, filtering, and switching.
C1 [Abbaslou, Siamak; Gatdula, Robert; Jiang, Wei] Rutgers State Univ, Dept Elect & Comp Engn, Piscataway, NJ 08854 USA.
[Lu, Ming; Stein, Aaron] Brookhaven Natl Lab, Ctr Funct Nanomat, Upton, NY 11973 USA.
[Soref, Richard A.] Univ Massachusetts, Dept Engn, Boston, MA 02125 USA.
RP Jiang, W (reprint author), Rutgers State Univ, Dept Elect & Comp Engn, Piscataway, NJ 08854 USA.
EM s.abaslou@rutgers.edu; rgatdula@rutgers.edu; mlu@bnl.gov; stein@bnl.gov;
richard.soref@umb.edu; wjiangnj@rci.rutgers.edu
OI Abbaslou, Siamak/0000-0003-4204-7002
NR 24
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U1 6
U2 9
PU IEEE-INST ELECTRICAL ELECTRONICS ENGINEERS INC
PI PISCATAWAY
PA 445 HOES LANE, PISCATAWAY, NJ 08855-4141 USA
SN 1041-1135
EI 1941-0174
J9 IEEE PHOTONIC TECH L
JI IEEE Photonics Technol. Lett.
PD OCT 15
PY 2016
VL 28
IS 20
BP 2137
EP 2140
DI 10.1109/LPT.2016.2582641
PG 4
WC Engineering, Electrical & Electronic; Optics; Physics, Applied
SC Engineering; Optics; Physics
GA DV2TI
UT WOS:000382773900006
ER
PT J
AU Wang, YX
Yan, PF
Xiao, J
Lu, XC
Zhang, JG
Sprenkle, VL
AF Wang, Yuxing
Yan, Pengfei
Xiao, Jie
Lu, Xiaochuan
Zhang, Ji-Guang
Sprenkle, Vincent L.
TI Effect of Al2O3 on the sintering of garnet-type Li6.5La3Zr1.5Ta0.5O12
SO SOLID STATE IONICS
LA English
DT Article
DE Garnet oxide; Lithium ion conductor; Solid electrolyte; Liquid-phase
sintering; Al2O3
ID STATE LITHIUM BATTERIES; HIGH IONIC-CONDUCTIVITY; SOLID ELECTROLYTES;
CONDUCTORS LI7LA3ZR2O12; SUPERIONIC CONDUCTOR; TRANSPORT-PROPERTIES; LI
BATTERIES; AL; TA; LI-7-XLA3ZR2-XTAXO12
AB It is widely recognized that Al plays a dual role in the fabrication of garnet-type solid electrolytes, i.e., as a dopant that stabilizes the cubic structure and a sintering aid that facilitates the densification. However, the sintering effect of Al2O3 has not been well understood so far because Al is typically "unintentionally" introduced into the sample from the crucible during the fabrication process. In this study, we have investigated the sintering effect of Al on the phase composition, microstructure, and ionic conductivity of Li6.5La3Zr1.5Ta0.5O12 by using an Al-free crucible and intentionally adding various amounts of gamma-Al2O3. It was found that the densification of Li6.5La3Zr1.5Ta0.5O12 occurred via liquid-phase sintering, with evidence of morphology change among different compositions. Among all of the compositions, samples with 0.05 mol Al per unit formula of garnet oxide (i.e., 0.3 wt% Al2O3) exhibited the optimal microstructure and the highest total ionic conductivity of 5 x 10(-4) S cm(-1) at room temperature. (C) 2016 Elsevier B.V. All rights reserved.
C1 [Wang, Yuxing; Yan, Pengfei; Xiao, Jie; Lu, Xiaochuan; Zhang, Ji-Guang; Sprenkle, Vincent L.] Pacific NW Natl Lab, Richland, WA 99352 USA.
RP Lu, XC (reprint author), Pacific NW Natl Lab, Richland, WA 99352 USA.
EM Xiaochuan.Lu@pnnl.gov
RI yan, pengfei/E-4784-2016; Wang, Yuxing/F-3195-2017
OI yan, pengfei/0000-0001-6387-7502; Wang, Yuxing/0000-0002-7828-9399
FU U.S. Department of Energy's (DOE's) Office of Electricity Delivery &
Energy Reliability (OE) [57558]; DOE [DE-AC05-76RL01830]
FX This work was supported by the U.S. Department of Energy's (DOE's) (No.
57558) Office of Electricity Delivery & Energy Reliability (OE). We
appreciate the useful discussions with Dr. I. Gyuk of the DOE-OE Grid
Storage Program. PNNL is a multiprogram laboratory operated by Battelle
Memorial Institute for the DOE under Contract DE-AC05-76RL01830.
NR 52
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U1 81
U2 86
PU ELSEVIER SCIENCE BV
PI AMSTERDAM
PA PO BOX 211, 1000 AE AMSTERDAM, NETHERLANDS
SN 0167-2738
EI 1872-7689
J9 SOLID STATE IONICS
JI Solid State Ion.
PD OCT 15
PY 2016
VL 294
BP 108
EP 115
DI 10.1016/j.ssi.2016.06.013
PG 8
WC Chemistry, Physical; Physics, Condensed Matter
SC Chemistry; Physics
GA DU6VC
UT WOS:000382351700014
ER
PT J
AU Li, J
Stinis, P
AF Li, Jing
Stinis, Panos
TI A unified framework for mesh refinement in random and physical space
SO JOURNAL OF COMPUTATIONAL PHYSICS
LA English
DT Article
DE Adaptive mesh refinement; Multi-element; gPC; Uncertainty
quantification; Discontinuities
ID PARTIAL-DIFFERENTIAL-EQUATIONS; STOCHASTIC COLLOCATION METHOD; RANDOM
INPUT DATA; GENERALIZED POLYNOMIAL CHAOS; UNCERTAINTY QUANTIFICATION;
ELLIPTIC PROBLEMS; APPROXIMATIONS; COEFFICIENTS; EXPANSIONS; ORDER
AB In recent work we have shown how an accurate reduced model can be utilized to perform mesh refinement in random space. That work relied on the explicit knowledge of an accurate reduced model which is used to monitor the transfer of activity from the large to the small scales of the solution. Since this is not always available, we present in the current work a framework which shares the merits and basic idea of the previous approach but does not require an explicit knowledge of a reduced model. Moreover, the current framework can be applied for refinement in both random and physical space. In this manuscript we focus on the application to random space mesh refinement. We study examples of increasing difficulty (from ordinary to partial differential equations) which demonstrate the efficiency and versatility of our approach. We also provide some results from the application of the new framework to physical space mesh refinement. (C) 2016 Elsevier Inc. All rights reserved.
C1 [Li, Jing; Stinis, Panos] Pacific Northwest Natl Lab, Richland, WA 99352 USA.
RP Li, J (reprint author), Pacific Northwest Natl Lab, Richland, WA 99352 USA.
EM jing.li@pnnl.gov; panagiotis.stinis@pnnl.gov
FU U.S. Department of Energy Office of Science, Office of Advanced
Scientific Computing Research, Applied Mathematics program,
Collaboratory on Mathematics for Mesoscopic Modeling of Materials (CM4)
[DE-SC0009280]
FX We would like to thank Prof. G. Karniadakis and Dr. F. Song for helpful
discussions and comments. This material is based upon work supported by
the U.S. Department of Energy Office of Science, Office of Advanced
Scientific Computing Research, Applied Mathematics program,
Collaboratory on Mathematics for Mesoscopic Modeling of Materials (CM4),
under Award Number DE-SC0009280.
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U1 2
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PU ACADEMIC PRESS INC ELSEVIER SCIENCE
PI SAN DIEGO
PA 525 B ST, STE 1900, SAN DIEGO, CA 92101-4495 USA
SN 0021-9991
EI 1090-2716
J9 J COMPUT PHYS
JI J. Comput. Phys.
PD OCT 15
PY 2016
VL 323
BP 243
EP 264
DI 10.1016/j.jcp.2016.07.027
PG 22
WC Computer Science, Interdisciplinary Applications; Physics, Mathematical
SC Computer Science; Physics
GA DT6HO
UT WOS:000381585500013
ER
PT J
AU Zhang, L
Mao, JF
Shi, XY
Ricciuto, D
He, HL
Thornton, P
Yu, GR
Li, P
Liu, M
Ren, XL
Han, SJ
Li, YN
Yan, JH
Hao, YB
Wang, HM
AF Zhang, Li
Mao, Jiafu
Shi, Xiaoying
Ricciuto, Daniel
He, Honglin
Thornton, Peter
Yu, Guirui
Li, Pan
Liu, Min
Ren, Xiaoli
Han, Shijie
Li, Yingnian
Yan, Junhua
Hao, Yanbin
Wang, Huimin
TI Evaluation of the Community Land Model simulated carbon and water fluxes
against observations over ChinaFLUX sites
SO AGRICULTURAL AND FOREST METEOROLOGY
LA English
DT Article
DE Community land model; ChinaFLUX; Eddy covariance; Carbon flux
ID AIR CO2 ENRICHMENT; GLOBAL VEGETATION MODELS; LEYMUS-CHINENSIS STEPPE;
NET ECOSYSTEM EXCHANGE; EARTH SYSTEM MODELS; CYCLE FEEDBACKS; FOREST
ECOSYSTEMS; USE EFFICIENCY; CONIFEROUS PLANTATION; UNCERTAINTY ANALYSIS
AB The Community Land Model (CLM) is an advanced process-based land surface model that simulates carbon, nitrogen, water vapor and energy exchanges between terrestrial ecosystems and the atmosphere at various spatial and temporal scales. We use observed carbon and water fluxes from five representative Chinese Terrestrial Ecosystem Flux Research Network (ChinaFLUX) eddy covariance tower sites to systematically evaluate the new version CLM4.5 and old version CLM4.0, and to generate insights that may inform future model developments. CLM4.5 underestimates the annual carbon sink at three forest sites and one alpine grassland site but overestimates the carbon sink of a semi-arid grassland site. The annual carbon sink underestimation for the deciduous-dominated forest site results from underestimated daytime carbon sequestration during summer and overestimated nighttime carbon emission during spring and autumn. Compared to CLM4.0, the bias of annual gross primary production (GPP) is reduced by 24% and 28% in CLM4.5 at two subtropical forest sites. However, CLM4.5 still presents a large positive bias in annual GPP. The improvement in net ecosystem exchange (NEE) is limited, although soil respiration bias decreases by 16%-43% at three forest sites. CLM4.5 simulates lower soil water content in the dry season than CLM4.0 at two grassland sites. Drier soils produce a significant drop in the leaf area index and in GPP and an increase in respiration for CLM4.5. The new fire parameterization approach in CLM4.5 causes excessive burning at the Changbaishan forest site, resulting in an unexpected underestimation of NEE, vegetation carbon, and soil organic carbon by 46%, 95%, and 87%, respectively. Overall, our study reveals significant improvements achieved by CLM4.5 compared to CLM4.0, and suggests further developments on the parameterization of seasonal GPP and respiration, which will require a more effective representation of seasonal water conditions and the partitioning of net radiation between sensible and heat fluxes. (C) 2016 Elsevier B.V. All rights reserved.
C1 [Zhang, Li; He, Honglin; Yu, Guirui; Ren, Xiaoli; Wang, Huimin] Chinese Acad Sci, Inst Geog Sci & Nat Resources Res, Key Lab Ecosyst Network Observat & Modeling, Beijing 100101, Peoples R China.
[Mao, Jiafu; Shi, Xiaoying; Ricciuto, Daniel; Thornton, Peter] Oak Ridge Natl Lab, Div Environm Sci, Oak Ridge, TN USA.
[Mao, Jiafu; Shi, Xiaoying; Ricciuto, Daniel; Thornton, Peter] Oak Ridge Natl Lab, Climate Change Sci Inst, Oak Ridge, TN USA.
[Li, Pan] Chinese Acad Sci, Inst Geochem, Guiyang 550081, Peoples R China.
[Liu, Min] E China Normal Univ, Shanghai Key Lab Urban Ecol & Sustainabil, Shanghai 200062, Peoples R China.
[Han, Shijie] Chinese Acad Sci, Inst Appl Ecol, Shenyang 110016, Peoples R China.
[Li, Yingnian] Chinese Acad Sci, Northwest Inst Plateau Biol, Xining 810001, Peoples R China.
[Yan, Junhua] Chinese Acad Sci, South China Bot Garden, Guangzhou 510650, Guangdong, Peoples R China.
[Hao, Yanbin] Univ Chinese Acad Sci, Beijing 100049, Peoples R China.
RP Yu, GR (reprint author), Chinese Acad Sci, Inst Geog Sci & Nat Resources Res, Key Lab Ecosyst Network Observat & Modeling, Beijing 100101, Peoples R China.
EM yugr@igsnrr.ac.cn
RI 于, 贵瑞/C-1768-2014; Mao, Jiafu/B-9689-2012; Thornton, Peter/B-9145-2012;
Ricciuto, Daniel/I-3659-2016
OI Mao, Jiafu/0000-0002-2050-7373; Thornton, Peter/0000-0002-4759-5158;
Ricciuto, Daniel/0000-0002-3668-3021
FU National Key Research and development program of China [2015CB954102];
National Natural Science Foundation of China [31290221, 31420103917];
Strategic Priority Research Program of the Chinese Academy of Sciences
[XDA05050602]; US Department of Energy (DOE), Office of Science,
Biological and Environmental Research; DOE [DE-AC05-00OR22725]
FX This work was financially supported by the National Key Research and
development program of China (2015CB954102), the National Natural
Science Foundation of China (31290221, 31420103917), and the Strategic
Priority Research Program of the Chinese Academy of Sciences
(XDA05050602). We thank all related staff from ChinaFLUX and CERN for
their contributions from observations to data processing. This research
was supported in part by the US Department of Energy (DOE), Office of
Science, Biological and Environmental Research. The Oak Ridge National
Laboratory is managed by UT-BATTELLE for DOE under contract
DE-AC05-00OR22725.
NR 81
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U1 30
U2 47
PU ELSEVIER SCIENCE BV
PI AMSTERDAM
PA PO BOX 211, 1000 AE AMSTERDAM, NETHERLANDS
SN 0168-1923
EI 1873-2240
J9 AGR FOREST METEOROL
JI Agric. For. Meteorol.
PD OCT 15
PY 2016
VL 226
BP 174
EP 185
DI 10.1016/j.agrformet.2016.05.018
PG 12
WC Agronomy; Forestry; Meteorology & Atmospheric Sciences
SC Agriculture; Forestry; Meteorology & Atmospheric Sciences
GA DS2KK
UT WOS:000380598200015
ER
PT J
AU Dieterich, M
Kutchko, B
Goodman, A
AF Dieterich, Matthew
Kutchko, Barbara
Goodman, Angela
TI Characterization of Marcellus Shale and Huntersville Chert before and
after exposure to hydraulic fracturing fluid via feature relocation
using field-emission scanning electron microscopy
SO FUEL
LA English
DT Article
DE Geochemistry; Appalachian Basin; Marcellus Shale; Scanning electron
microscopy; Shale; Fluid-rock interaction
ID WATER-ROCK INTERACTIONS; GAS-WELLS; PENNSYLVANIA
AB Two sets of experimental in situ fluid rock interaction studies were implemented to understand the interactions between hydraulic fracturing fluid and rocks of the Marcellus Shale gas play. Marcellus Shale and Huntersville Chert core samples were exposed to synthetically prepared fracturing fluid and recycled fracturing fluid from the field, respectively, and examined before and after in situ exposure using surface relocation techniques via high-resolution field-emission scanning electron microscopy (FE-SEM) to investigate chemical or physical alterations.
Results indicate that in situ pressure promoted fracture growth along the sedimentological (horizontal) bedding plane of the Marcellus Shale samples. Moreover, calcium carbonate (CaCO3) dissolution was observed and gypsum (CaSO4 * 2H(2)O) appeared to precipitate both on the surface and in the numerous fractures. Barite (BaSO4), strontianite (SrCO3), celestine (SrSO4), and apatite (CaPO4) formed a unique pattern of precipitates on the surface of the Huntersville Chert samples. Additionally, Rhenium and rare earth element (REE) Europium were identified in minerals which precipitated on the Huntersville Chert surface identified by FE-SEM spectral analysis. Published by Elsevier Ltd.
C1 [Dieterich, Matthew; Kutchko, Barbara; Goodman, Angela] US DOE, Off Res & Dev, Natl Energy Technol Lab, 626 Cochrans Mill Rd, Pittsburgh, PA 15236 USA.
RP Kutchko, B (reprint author), US DOE, Off Res & Dev, Natl Energy Technol Lab, 626 Cochrans Mill Rd, Pittsburgh, PA 15236 USA.
EM Barbara.Kutchko@netl.doe.gov
FU U.S. Department of Energy
FX We would like to thank Rick Hammack for the recycled fracturing fluid
from the well pad in Greene Co. Pennsylvania and Brett Howard for X-ray
diffraction characterization of the Marcellus Shale and Huntersville
Chert core. Also, we would like to thank the reviewers who helped
improve our paper. This research was supported in part by appointments
to the National Energy Technology Laboratory Research Participation
Program, sponsored by the U.S. Department of Energy and administered by
the Oak Ridge Institute for Science and Education.
NR 28
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PU ELSEVIER SCI LTD
PI OXFORD
PA THE BOULEVARD, LANGFORD LANE, KIDLINGTON, OXFORD OX5 1GB, OXON, ENGLAND
SN 0016-2361
EI 1873-7153
J9 FUEL
JI Fuel
PD OCT 15
PY 2016
VL 182
BP 227
EP 235
DI 10.1016/j.fuel.2016.05.061
PG 9
WC Energy & Fuels; Engineering, Chemical
SC Energy & Fuels; Engineering
GA DQ3LA
UT WOS:000379102600025
ER
PT J
AU Jarvis, JM
Sudasinghe, NM
Albrecht, KO
Schmidt, AJ
Hallen, RT
Anderson, DB
Billing, JM
Schaub, TM
AF Jarvis, Jacqueline M.
Sudasinghe, Nilusha M.
Albrecht, Karl O.
Schmidt, Andrew J.
Hallen, Richard T.
Anderson, Daniel B.
Billing, Justin M.
Schaub, Tanner M.
TI Impact of iron porphyrin complexes when hydroprocessing algal HTL
biocrude
SO FUEL
LA English
DT Article
DE ICR; FT-ICR MS; HTL biocrude; Porphyrins; ICP; Algae; Iron porphyrins;
Biofuel; Thermochemical processing
ID ICR MASS-SPECTROMETRY; HEAVY CRUDE-OIL; HYDROTHERMAL LIQUEFACTION;
VANADYL PORPHYRINS; NICKEL PORPHYRINS; CATALYTIC HYDRODEMETALLATION;
MOLECULAR CHARACTERIZATION; NATURAL SEEPS; CHROMATOGRAPHY;
PETROPORPHYRINS
AB We apply Fourier transform ion cyclotron resonance mass spectrometry (FT-ICR MS) for direct characterization of iron-porphyrins in hydrothermal liquefaction (HTL) biocrude oils derived from two algae: Tetraselmis sp. and cyanobacteria. The iron porphyrin compounds are shown to cause catalyst bed plugging during hydroprocessing due to iron deposition. Inductively-coupled plasma optical emission spectrometry (ICP-OES) was utilized for iron quantitation in the plugged catalyst beds formed through hydroprocessing of the two HTL biocrudes and identifies an enrichment of iron in the upper five centimeters of the catalyst bed for Tetraselmis sp. (Fe = 100,728 ppm) and cyanobacteria (Fe = 115,450 ppm). Direct infusion FT-ICR MS analysis of the two HTL biocrudes with optimized instrument conditions facilitates rapid screening and identification of iron porphyrins without prior chromatographic separation. With FT-ICR MS we identify 138 unique iron porphyrin compounds in the two HTL biocrudes that have similar carbon number and double bond equivalent distributions to the metal porphyrins (e.g. Ni and V) reported for petroleum. No iron porphyrins are Observed in the cyanobacteria HTL biocrude after hydroprocessing, which indicates that iron porphyrin structures in the HTL biocrude are degraded during hydrotreatment. Hydrodemetallization reactions that occur through hydroprocessing of HTL biocrudes could be responsible for the decomposition of iron porphyrin structures leading to metal deposition in the catalyst bed that result in catalyst deactivation and bed plugging, and must be addressed for effective upgrading of algal HTL biocrudes. (C) 2016 Elsevier Ltd. All rights reserved.
C1 [Jarvis, Jacqueline M.; Sudasinghe, Nilusha M.; Schaub, Tanner M.] New Mexico State Univ, Coll Agr Consumer & Environm Sci, Chem Anal & Instrumentat Lab, 945 Coll Ave, Las Cruces, NM 88003 USA.
[Albrecht, Karl O.; Schmidt, Andrew J.; Hallen, Richard T.; Anderson, Daniel B.; Billing, Justin M.] Pacific NW Natl Lab, Chem & Biol Proc Dev Grp, POB 999, Richland, WA 99352 USA.
RP Schaub, TM (reprint author), New Mexico State Univ, Coll Agr Consumer & Environm Sci, Chem Anal & Instrumentat Lab, 945 Coll Ave, Las Cruces, NM 88003 USA.
EM tschaub@nmsu.edu
OI Billing, Justin/0000-0003-1442-8916
FU United States National Science Foundation [IIA-1301346]; Center for
Animal Health and Food Safety at New Mexico State University; U.S.
Department of Energy's Office of Energy Efficiency and Renewable Energy
(Bioenergy Technologies Office)
FX This work was supported by the U.S. Department of Energy's Office of
Energy Efficiency and Renewable Energy (Bioenergy Technologies Office),
the United States National Science Foundation (IIA-1301346) and the
Center for Animal Health and Food Safety at New Mexico State University.
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PU ELSEVIER SCI LTD
PI OXFORD
PA THE BOULEVARD, LANGFORD LANE, KIDLINGTON, OXFORD OX5 1GB, OXON, ENGLAND
SN 0016-2361
EI 1873-7153
J9 FUEL
JI Fuel
PD OCT 15
PY 2016
VL 182
BP 411
EP 418
DI 10.1016/j.fuel.2016.05.107
PG 8
WC Energy & Fuels; Engineering, Chemical
SC Energy & Fuels; Engineering
GA DQ3LA
UT WOS:000379102600044
ER
PT J
AU Ferris, AM
Rothamer, DA
AF Ferris, Alison M.
Rothamer, David A.
TI Methodology for the experimental measurement of vapor-liquid equilibrium
distillation curves using a modified ASTM D86 setup
SO FUEL
LA English
DT Article
DE ASTM D86; Distillation curve; Dynamic holdup; Vapor-liquid equilibrium;
Experimental equilibrium distillation curve; EEDC
ID EXTENSION; REVISION
AB A method has been developed to determine experimental equilibrium distillation curves using a modified ASTM D86 distillation apparatus.The method determines accurate equilibrium initial boiling points and accounts for the dynamic holdup inherent in distillation curves measured in accordance with the ASTM D86 standard.In this work, the ASTM D86 distillation setup has been modified to simultaneously measure liquid and vapor temperature using two resistance temperature detectors (RTDs) and a data acquisition system has been employed to record temperature data at one-second time intervals for the duration of each distillation.Additionally, the time for each volume recovery point is recorded.The method presented here uses the time-resolved liquid temperature data to identify the true initial boiling point (IBP) of four fuel mixtures of known composition; the IBPs are within 2 degrees C of the calculated equilibrium values.The time-resolved volume recovery information and the identified initial boiling point time are used to construct a volume evaporated versus time curve.The measured temperatures determined at the corresponding volume evaporated increments provide an experimental equilibrium distillation curve (EEDC). The EEDCs for the four fuel mixtures of known composition match the calculated equilibrium curves within a few degrees Celsius; a maximum mean absolute error of 2.2 +/- 1.4 degrees C was observed.The dynamic holdup (volume difference between volume evaporated and volume recovered) associated with a distillation is found to correlate with the initial boiling point of the fuel being distilled and the temperature of the condenser bath used in the experiment.The method was also applied to measure EEDCs for a gasoline fuel and a diesel fuel, where the compositions were unknown, to investigate the differences between the EEDCs and the ASTM D86 distillation curves.The results highlight the large errors incurred when using ASTM D86 results to approximate equilibrium distillation curves. (C) 2016 The Authors. Published by Elsevier Ltd. This is an open access article under the CC BY-NC-ND.
C1 [Rothamer, David A.] Univ Wisconsin, Dept Mech Engn, 1500 Engn Dr, Madison, WI 53706 USA.
Univ Wisconsin, DOE Great Lakes Bioenergy Res Ctr, 1500 Engn Dr, Madison, WI 53706 USA.
RP Rothamer, DA (reprint author), Univ Wisconsin, Dept Mech Engn, 1500 Engn Dr, Madison, WI 53706 USA.
EM rothamer@wisc.edu
FU U.S. Department of Energy Great Lakes Bioenergy Research Center (DOE BER
Office of Science) [DE-FC02-07ER64494]
FX This work was funded by the U.S. Department of Energy Great Lakes
Bioenergy Research Center (DOE BER Office of Science DE-FC02-07ER64494).
NR 20
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U1 4
U2 8
PU ELSEVIER SCI LTD
PI OXFORD
PA THE BOULEVARD, LANGFORD LANE, KIDLINGTON, OXFORD OX5 1GB, OXON, ENGLAND
SN 0016-2361
EI 1873-7153
J9 FUEL
JI Fuel
PD OCT 15
PY 2016
VL 182
BP 467
EP 479
DI 10.1016/j.fue1.2016.05.099
PG 13
WC Energy & Fuels; Engineering, Chemical
SC Energy & Fuels; Engineering
GA DQ3LA
UT WOS:000379102600050
ER
PT J
AU Shi, SW
Weber, AZ
Kusoglu, A
AF Shi, Shouwen
Weber, Adam Z.
Kusoglu, Ahmet
TI Structure/property relationship of Nafion XL composite membranes
SO JOURNAL OF MEMBRANE SCIENCE
LA English
DT Article
DE Nafion XL; Composite membranes; Structure/property; SAXS/WAXS; PEM fuel
cells
ID POLYMER ELECTROLYTE MEMBRANE; PROTON-EXCHANGE MEMBRANES; FUEL-CELL
MEMBRANES; SULFONIC-ACID MEMBRANE; CHEMICAL DEGRADATION; MECHANICAL
DURABILITY; RELAXATION PHENOMENA; HUMIDITY CYCLES; PFSA MEMBRANES;
THROUGH-PLANE
AB Perfluorosulfonic-acid (PFSA) ionomer membranes (most commonly Nafion (R)) are currently the prototypical proton-exchange-membrane in polymer-electrolyte fuel cells (PEFCs), for which durability still represents a technical barrier to their commercialization. In an effort to address the durability demands, PFSA membranes with reinforcement and/or stabilizers have become of great interest as they have demonstrated superior durability in PEFCs compared to their unreinforced analogues. One such particular membrane that is tailored for enhanced durability and commonly employed in PEFCs is Nafion XL, a Nafion-based ionomer membrane with mechanical reinforcement and chemical stabilizers. Despite an increasing number of recent studies demonstrating its improved lifetime in accelerated stress testing (AST), its structure and transport properties have not been investigated in a systematic fashion. In this paper, we report water uptake, dimensional change, conductivity, and mechanical properties of Nafion XL membrane, as well as its strong anisotropy, in comparison to (unreinforced) Nafion 212 membrane. Moreover, water-domain spacing and crystallinity of Nafion XL membrane, determined from small- and wide-angle X-ray scattering (SAXS/WAXS) experiments, are correlated with the measured properties to establish a structure/property relationship, and discussed within the context of composite materials. It is also found that (pre)conditioning of the membrane by heating in water at different temperatures could have significant impacts on its structure/property relationship, in particular, the mechanical stability and conductivity, and their anisotropy, which were related to morphological changes observed from microscopy studies. The findings reported here not only provide a new dataset that can be used for PEFC performance and durability modeling but also benefit the efforts on developing composite ion-conductive membranes. (C) 2016 Elsevier B.V. All rights reserved.
C1 [Shi, Shouwen; Weber, Adam Z.; Kusoglu, Ahmet] Lawrence Berkeley Natl Lab, Energy Technol Area, 1 Cyclotron Rd, Berkeley, CA 94720 USA.
[Shi, Shouwen] Tianjin Univ, Sch Chem Engn & Technol, Tianjin 300072, Peoples R China.
RP Kusoglu, A (reprint author), Lawrence Berkeley Natl Lab, Energy Technol Area, 1 Cyclotron Rd, Berkeley, CA 94720 USA.
EM akusaglu@lbl.gov
OI Kusoglu, Ahmet/0000-0002-2761-1050
FU Department of Energy, Office of Basic Energy Sciences
[DE-AC02-05CH11231]; China Scholarship Council (CSC); Fuel Cell
Performance and Durability Consortium (FC-PAD); Fuel Cell Technologies
Office (FCTO); Office of Energy Efficiency and Renewable Energy (EERE);
U.S. Department of Energy [DE-AC02-05CH11231]
FX The authors also acknowledge Karren More of Oak Ridge National Lab
(ORNL) for taking and providing the STEM images, and Grace Lau (LBNL)
for the SEM studies. AK and AZW would like to thank Rod Borup and
Rangachary Mukundan of Los Alamos National Laboratory (LANL) for
insightful discussions. SAXS/WAXS experiments were performed in the
beamline 7.3.3 at Advanced Light Source (ALS), Lawrence Berkeley
National Laboratory, which is a national user facility funded by the
Department of Energy, Office of Basic Energy Sciences under the contract
number DE-AC02-05CH11231. We thank Chenhui Zhu and Dr. Eric Schiable for
their assistance during facilitating the use of equipment at ALS.
Shouwen Shi greatly thanks China Scholarship Council (CSC) for financial
support during his visit to Lawrence Berkeley National Laboratory. This
work was funded under the Fuel Cell Performance and Durability
Consortium (FC-PAD), by the Fuel Cell Technologies Office (FCTO), Office
of Energy Efficiency and Renewable Energy (EERE), of the U.S. Department
of Energy under contract number DE-AC02-05CH11231 and Program
Development Managers Dimitrios Papageorgopoulos and Greg Kleen.
NR 66
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U1 24
U2 73
PU ELSEVIER SCIENCE BV
PI AMSTERDAM
PA PO BOX 211, 1000 AE AMSTERDAM, NETHERLANDS
SN 0376-7388
EI 1873-3123
J9 J MEMBRANE SCI
JI J. Membr. Sci.
PD OCT 15
PY 2016
VL 516
BP 123
EP 134
DI 10.1016/j.memsci.2016.06.004
PG 12
WC Engineering, Chemical; Polymer Science
SC Engineering; Polymer Science
GA DR1YB
UT WOS:000379699700013
ER
PT J
AU Liu, LW
Zhang, LR
Liang, LY
Ohsasa, K
Koyama, T
Sheng, Q
Hasegawa, T
Ishio, S
AF Liu, Liwang
Zhang, Luran
Liang, Linyun
Ohsasa, Kenichi
Koyama, Toshiyuki
Sheng, Qiang
Hasegawa, Takashi
Ishio, Shunji
TI Microstructure of L1(0) FePt thin films with anisotropic interfacial
energy coefficients and anisotropic atomic mobilities
SO JOURNAL OF ALLOYS AND COMPOUNDS
LA English
DT Article
DE FePt; Anisotropic mobility; Anisotropic interfacial energy coefficients;
Columnar microstructure; Phase field
ID EVOLUTION; SIZE
AB The microstructure evolutions of FePt-X (segregant) thin films were studied by employing a three-dimensional phase field model. Simulated results show that in the absence of substrate constraint related with elastic energy, the morphology of the FePt-X thin films significantly depends on the film thickness, anisotropic interfacial energy coefficients, and anisotropic atomic mobility. Small in-plane anisotropic interfacial energy coefficients or out-of-plane anisotropic mobility of atom diffusion are beneficial to induce columnar shape FePt grains, using any one of parameters of which can make the FePt grains keep columnar shape when FePt-X thin films thickness is 10 nm. Using segregant with both proper in-plane anisotropic interfacial energy coefficients and out-of-plane anisotropic mobility can make the FePt grains keep columnar shape when the FePt-X thin films thickness reaches to at least 15 nm. (C) 2016 Elsevier B.V. All rights reserved.
C1 [Liu, Liwang; Zhang, Luran; Ishio, Shunji] Akita Univ, Venture Business Lab, Gakuen Machi 1-1, Akita 0108502, Japan.
[Liang, Linyun] Argonne Natl Lab, Math & Comp Sci Div, 9700 S Cass Ave, Argonne, IL 60439 USA.
[Ohsasa, Kenichi; Hasegawa, Takashi; Ishio, Shunji] Akita Univ, Dept Mat Sci & Engn, Gakuen Machi 1-1, Akita 0108502, Japan.
[Koyama, Toshiyuki] Nagoya Univ, Grad Sch Engn, Dept Mat Phys & Energy Engn, Chikusa Ku, Furo Cho, Nagoya, Aichi 4648603, Japan.
[Sheng, Qiang] Harbin Inst Technol, Shenzhen Grad Sch, Dept Mat Sci & Engn, Shenzhen 518055, Peoples R China.
RP Ishio, S (reprint author), Akita Univ, Dept Mat Sci & Engn, Gakuen Machi 1-1, Akita 0108502, Japan.
EM ishio@gipc.akita-u.ac.jp
FU Japan Science and Technology Agency (JST)
FX This work was supported by the Japan Science and Technology Agency (JST)
under collaborative research based on industrial demand "High
performance magnets: towards innovative development of next generation
magnets".
NR 18
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U1 6
U2 7
PU ELSEVIER SCIENCE SA
PI LAUSANNE
PA PO BOX 564, 1001 LAUSANNE, SWITZERLAND
SN 0925-8388
EI 1873-4669
J9 J ALLOY COMPD
JI J. Alloy. Compd.
PD OCT 15
PY 2016
VL 682
BP 176
EP 179
DI 10.1016/j.jallcom.2016.04.261
PG 4
WC Chemistry, Physical; Materials Science, Multidisciplinary; Metallurgy &
Metallurgical Engineering
SC Chemistry; Materials Science; Metallurgy & Metallurgical Engineering
GA DP9RB
UT WOS:000378833400023
ER
PT J
AU Svanidze, E
Kindy, M
Georgen, C
Fulfer, BW
Lapidus, SH
Chan, JY
Morosan, E
AF Svanidze, E.
Kindy, M., II
Georgen, C.
Fulfer, B. W.
Lapidus, S. H.
Chan, J. Y.
Morosan, E.
TI Magnetic and crystallographic properties of ZrM2-delta Zn20+delta
(M=Cr-Cu)
SO JOURNAL OF MAGNETISM AND MAGNETIC MATERIALS
LA English
DT Article
DE Magnetism; Itinerant magnetism; Transition metal; Intermetallics;
Magnetic moment dilution; Cubic Laves phases
ID LOCAL MOMENT; CRYSTAL-STRUCTURE; LAVES PHASES; ELECTRON; ZR; CO;
FERROMAGNETISM; DEGENERACY; TRANSITION; COMPOUND
AB Single crystals of the cubic Laves ternaries ZrM2-delta Zn20+delta (M=Mn, Fe, Co, Ni and Cu, 0 <= delta <= 1) have been synthesized using a self-flux method. The magnetic properties of these compounds were compared with structurally similar cubic binaries ZrM2 (M=Mn, Fe, Co, Ni and Cu). A transition from local to itinerant moment magnetism was observed for M=Fe and M=Mn, while all other ternaries exhibit weakly para- or diamagnetic behavior. The local-to-itinerant crossover can be explained by a nearly two-fold increase of the M-M bond length d(M-M) in ZrM2-delta Zn20+delta compounds, as compared with the ZrM2 binaries. Additionally, we report two new compounds in this series ZrCrZn21 and ZrCu2Zn20. Analysis of crystallographic and magnetic trends in these materials will aid in understanding of magnetism in general and 3d intermetallics in particular. (C) 2016 Elsevier B.V. All rights reserved.
C1 [Svanidze, E.; Kindy, M., II; Georgen, C.; Morosan, E.] Rice Univ, Dept Phys & Astron, Houston, TX 77005 USA.
[Fulfer, B. W.; Chan, J. Y.] Univ Texas Dallas, Dept Chem, Richardson, TX 75080 USA.
[Lapidus, S. H.] Argonne Natl Lab, Adv Photon Source, Xray Sci Div, Argonne, IL 60439 USA.
RP Morosan, E (reprint author), Max Planck Inst Chem Phys, Gottingen, Germany.
EM eteri@alumni.rice.edu; emorosan@rice.edu
RI Chan, Julia/C-5392-2008;
OI Chan, Julia/0000-0003-4434-2160; Svanidze, Eteri/0000-0003-2893-1379
FU NSF [DMR-1506704, DMR-1063735, DMR-1360863]
FX The work at Rice was supported by NSF DMR-1506704. J.Y.C. acknowledges
NSF DMR-1063735 and DMR-1360863 for partial support of this project.
NR 45
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U1 4
U2 15
PU ELSEVIER SCIENCE BV
PI AMSTERDAM
PA PO BOX 211, 1000 AE AMSTERDAM, NETHERLANDS
SN 0304-8853
EI 1873-4766
J9 J MAGN MAGN MATER
JI J. Magn. Magn. Mater.
PD OCT 15
PY 2016
VL 416
BP 401
EP 407
DI 10.1016/j.jmmm.2016.04.082
PG 7
WC Materials Science, Multidisciplinary; Physics, Condensed Matter
SC Materials Science; Physics
GA DN9IF
UT WOS:000377392100056
ER
PT J
AU Mu, L
Wang, JP
Ye, X
AF Mu, Lin
Wang, Junping
Ye, Xiu
TI A weak Galerkin generalized multiscale finite element method
SO JOURNAL OF COMPUTATIONAL AND APPLIED MATHEMATICS
LA English
DT Article
DE Weak Galerkin; Multiscale; Finite element methods; Elliptic problems
with rapidly oscillating or high contrast coefficients; Polyhedral
meshes
ID 2ND-ORDER ELLIPTIC PROBLEMS; INTERFACE PROBLEMS; POLYTOPAL MESHES;
POROUS-MEDIA; EQUATIONS
AB In this paper, we propose a general framework for weak Galerkin generalized multiscale (WG-GMS) finite element method for the elliptic problems with rapidly oscillating or high contrast coefficients. This general WG-GMS method features in high order accuracy on general meshes and can work with multiscale basis derived by different numerical schemes. A special case is studied under this WG-GMS framework in which the multiscale basis functions are obtained by solving local problem with the weak Galerkin finite element method. Convergence analysis and numerical experiments are obtained for the special case. (C) 2016 Elsevier B.V. All rights reserved.
C1 [Mu, Lin] Oak Ridge Natl Lab, Comp Sci & Math Div, Oak Ridge, TN 37831 USA.
[Wang, Junping] Natl Sci Fdn, Div Math Sci, 4201 Wilson Blvd, Arlington, VA 22230 USA.
[Ye, Xiu] Univ Arkansas, Dept Math, Little Rock, AR 72204 USA.
RP Mu, L (reprint author), Oak Ridge Natl Lab, Comp Sci & Math Div, Oak Ridge, TN 37831 USA.
EM mul1@ornl.gov; jwang@nsf.gov; xxye@ualr.edu
FU National Science Foundation [DMS-1418973, DMS-1115097]; Householder
Fellowship - U.S. Department of Energy, Office of Science, Office of
Advanced Scientific Computing Research, Applied Mathematics program
[ERKJE45]; Householder Fellowship - Laboratory Directed Research and
Development program at the Oak Ridge National Laboratory (ORNL); U.S.
Department of Energy [DE-AC05-00OR22725]; NSF IR/D program
FX The study of first author was supported in part by National Science
Foundation Grant DMS-1418973 and the Householder Fellowship which is
jointly funded by: the U.S. Department of Energy, Office of Science,
Office of Advanced Scientific Computing Research, Applied Mathematics
program, under award number ERKJE45, and the Laboratory Directed
Research and Development program at the Oak Ridge National Laboratory
(ORNL), which is operated by UT-Battelle, LLC., for the U.S. Department
of Energy under Contract DE-AC05-00OR22725. The research of Wang was
supported by the NSF IR/D program, while working at National Science
Foundation. However, any opinion, finding, and conclusions or
recommendations expressed in this material are those of the author and
do not necessarily reflect the views of the National Science Foundation.
The research of third author was supported in part by National Science
Foundation Grant DMS-1115097.
NR 35
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Z9 0
U1 4
U2 16
PU ELSEVIER SCIENCE BV
PI AMSTERDAM
PA PO BOX 211, 1000 AE AMSTERDAM, NETHERLANDS
SN 0377-0427
EI 1879-1778
J9 J COMPUT APPL MATH
JI J. Comput. Appl. Math.
PD OCT 15
PY 2016
VL 305
BP 68
EP 81
DI 10.1016/j.cam.2016.03.017
PG 14
WC Mathematics, Applied
SC Mathematics
GA DN1AR
UT WOS:000376798700007
ER
PT J
AU Somnath, S
Collins, L
Matheson, MA
Sukumar, SR
Kalinin, SV
Jesse, S
AF Somnath, Suhas
Collins, Liam
Matheson, Michael A.
Sukumar, Sreenivas R.
Kalinin, Sergei V.
Jesse, Stephen
TI Imaging via complete cantilever dynamic detection: general dynamic mode
imaging and spectroscopy in scanning probe microscopy
SO NANOTECHNOLOGY
LA English
DT Article
DE scanning probe microscopy (SPM); Kelvin probe force microscopy (KPFM);
electrostatic force microscopy (EFM); principal component analysis
(PCA); big data; high performance computing (HPC)
ID ATOMIC-FORCE MICROSCOPY; FREQUENCY-MODULATION-DETECTION; EXCITATION;
MICROCANTILEVER; RECOGNITION; ACQUISITION; RESOLUTION
AB We develop and implement a multifrequency spectroscopy and spectroscopic imaging mode, referred to as general dynamic mode (GDM), that captures the complete spatially- and stimulus dependent information on nonlinear cantilever dynamics in scanning probe microscopy (SPM). GDM acquires the cantilever response including harmonics and mode mixing products across the entire broadband cantilever spectrum as a function of excitation frequency. GDM spectra substitute the classical measurements in SPM, e.g. amplitude and phase in lock-in detection. Here, GDM is used to investigate the response of a purely capacitively driven cantilever. We use information theory techniques to mine the data and verify the findings with governing equations and classical lock-in based approaches. We explore the dependence of the cantilever dynamics on the tip-sample distance, AC and DC driving bias. This approach can be applied to investigate the dynamic behavior of other systems within and beyond dynamic SPM. GDM is expected to be useful for separating the contribution of different physical phenomena in the cantilever response and understanding the role of cantilever dynamics in dynamic AFM techniques.
C1 [Somnath, Suhas; Collins, Liam; Kalinin, Sergei V.; Jesse, Stephen] Oak Ridge Natl Lab, Ctr Nanophase Mat Sci, Oak Ridge, TN 37831 USA.
[Somnath, Suhas; Collins, Liam; Kalinin, Sergei V.; Jesse, Stephen] Oak Ridge Natl Lab, Inst Funct Imaging Mat, Oak Ridge, TN 37831 USA.
[Matheson, Michael A.; Sukumar, Sreenivas R.] Oak Ridge Natl Lab, Natl Ctr Computat Sci Div, Oak Ridge, TN 37831 USA.
RP Somnath, S; Jesse, S (reprint author), Oak Ridge Natl Lab, Ctr Nanophase Mat Sci, Oak Ridge, TN 37831 USA.; Somnath, S; Jesse, S (reprint author), Oak Ridge Natl Lab, Inst Funct Imaging Mat, Oak Ridge, TN 37831 USA.
EM somnaths@ornl.gov; sjesse@ornl.gov
FU Center for Nanophase Materials Sciences; Laboratory Director's Research
and Development fund; Office of Science of the US DOE; Scientific User
Facilities Division, Office of Basic Energy Sciences, US Department of
Energy (DOE)
FX Research was conducted at and supported by (SS, LFC, SVK, and SJ) the
Center for Nanophase Materials Sciences, which is sponsored at Oak Ridge
National Laboratory by the Scientific User Facilities Division, Office
of Basic Energy Sciences, US Department of Energy (DOE). Research for
MAM and SRS was funded by the Laboratory Director's Research and
Development fund. This research used resources of the Oak Ridge
Leadership Computing Facility at the Oak Ridge National Laboratory,
which is supported by the Office of Science of the US DOE.
NR 69
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U1 1
U2 1
PU IOP PUBLISHING LTD
PI BRISTOL
PA TEMPLE CIRCUS, TEMPLE WAY, BRISTOL BS1 6BE, ENGLAND
SN 0957-4484
EI 1361-6528
J9 NANOTECHNOLOGY
JI Nanotechnology
PD OCT 14
PY 2016
VL 27
IS 41
AR 414003
DI 10.1088/0957-4484/27/41/414003
PG 11
WC Nanoscience & Nanotechnology; Materials Science, Multidisciplinary;
Physics, Applied
SC Science & Technology - Other Topics; Materials Science; Physics
GA EL1FY
UT WOS:000394367100001
PM 27607339
ER
PT J
AU McClure, RS
Overall, CC
McDermott, JE
Hill, EA
Markillie, LM
Mccue, LA
Taylor, RC
Ludwig, M
Bryant, DA
Beliaev, AS
AF McClure, Ryan S.
Overall, Christopher C.
McDermott, Jason E.
Hill, Eric A.
Markillie, Lye Meng
McCue, Lee Ann
Taylor, Ronald C.
Ludwig, Marcus
Bryant, Donald A.
Beliaev, Alexander S.
TI Network analysis of transcriptomics expands regulatory landscapes in
Synechococcus sp PCC 7002
SO NUCLEIC ACIDS RESEARCH
LA English
DT Article
ID INORGANIC CARBON TRANSPORT; LIGHT-REPRESSED TRANSCRIPT; NONCODING RNAS;
POSTTRANSCRIPTIONAL CONTROL; COEXPRESSION NETWORKS; SYNECHOCYSTIS
PCC6803; CYANOBACTERIA; GENE; IDENTIFICATION; ACCLIMATION
AB Cyanobacterial regulation of gene expression must contend with a genome organization that lacks apparent functional context, as the majority of cellular processes and metabolic pathways are encoded by genes found at disparate locations across the genome and relatively few transcription factors exist. In this study, global transcript abundance data from the model cyanobacterium Synechococcus sp. PCC 7002 grown under 42 different conditions was analyzed using Context-Likelihood of Relatedness (CLR). The resulting network, organized into 11 modules, provided insight into transcriptional network topology as well as grouping genes by function and linking their response to specific environmental variables. When used in conjunction with genome sequences, the network allowed identification and expansion of novel potential targets of both DNA binding proteins and sRNA regulators. These results offer a new perspective into the multi-level regulation that governs cellular adaptations of the fast-growing physiologically robust cyanobacterium Synechococcus sp. PCC 7002 to changing environmental variables. It also provides a methodological high-throughput approach to studying multi-scale regulatory mechanisms that operate in cyanobacteria. Finally, it provides valuable context for integrating systems-level data to enhance gene grouping based on annotated function, especially in organisms where traditional context analyses cannot be implemented due to lack of operon-based functional organization.
C1 [McClure, Ryan S.; Overall, Christopher C.; McDermott, Jason E.; Hill, Eric A.; Markillie, Lye Meng; McCue, Lee Ann; Taylor, Ronald C.; Beliaev, Alexander S.] Pacific Northwest Natl Lab, Div Biol Sci, Richland, WA 99352 USA.
[Ludwig, Marcus; Bryant, Donald A.] Penn State Univ, Dept Biochem & Mol Biol, State Coll, PA 16802 USA.
[Bryant, Donald A.] Montana State Univ, Dept Chem & Biochem, Bozeman, MT 59717 USA.
RP Beliaev, AS (reprint author), Pacific Northwest Natl Lab, Div Biol Sci, Richland, WA 99352 USA.
EM alex.beliaev@pnnl.gov
FU Genomic Science Program (GSP); Office of Biological and Environmental
Research (BER); U.S. Department of Energy (DOE); PNNL Foundational and
Biofuels Scientific Focus Area; Air Force Office of Scientific Research
Support [FA9550-05-1-0365 (MURI), FA9550-11-1-0148]; National Science
Foundation [MCB-1021725]; DOE by Battelle Memorial Institute
[DE-AC05-76RLO 1830]
FX Genomic Science Program (GSP); Office of Biological and Environmental
Research (BER); U.S. Department of Energy (DOE); PNNL Foundational and
Biofuels Scientific Focus Area [to A. B]; Air Force Office of Scientific
Research Support [FA9550-05-1-0365 (MURI), FA9550-11-1-0148]; National
Science Foundation [MCB-1021725 to D.A.B]; PNNL is operated for the DOE
by Battelle Memorial Institute under Contract DE-AC05-76RLO 1830.
Funding for open access charge: PNNL Foundational and Biofuels
Scientific Focus Area [to A.B].
NR 63
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Z9 2
U1 5
U2 5
PU OXFORD UNIV PRESS
PI OXFORD
PA GREAT CLARENDON ST, OXFORD OX2 6DP, ENGLAND
SN 0305-1048
EI 1362-4962
J9 NUCLEIC ACIDS RES
JI Nucleic Acids Res.
PD OCT 14
PY 2016
VL 44
IS 18
BP 8810
EP 8825
DI 10.1093/nar/gkw737
PG 16
WC Biochemistry & Molecular Biology
SC Biochemistry & Molecular Biology
GA EA9ET
UT WOS:000386945000028
PM 27568004
ER
PT J
AU Cotton, SJ
Miller, WH
AF Cotton, Stephen J.
Miller, William H.
TI A new symmetrical quasi-classical model for electronically non-adiabatic
processes: Application to the case of weak non-adiabatic coupling
SO JOURNAL OF CHEMICAL PHYSICS
LA English
DT Article
ID MOLECULAR-DYNAMICS; QUANTUM DYNAMICS; S-MATRIX; SIMULATIONS; EXCITATION;
SYSTEMS; ENERGY; TIME
AB Previous work has shown how a symmetrical quasi-classical (SQC) windowing procedure can be used to quantize the initial and final electronic degrees of freedom in the Meyer-Miller (MM) classical vibronic (i.e, nuclear + electronic) Hamiltonian, and that the approach provides a very good description of electronically non-adiabatic processes within a standard classical molecular dynamics framework for a number of benchmark problems. This paper explores application of the SQC/MM approach to the case of very weak non-adiabatic coupling between the electronic states, showing (as anticipated) how the standard SQC/MM approach used to date fails in this limit, and then devises a new SQC windowing scheme to deal with it. Application of this new SQC model to a variety of realistic benchmark systems shows that the new model not only treats the weak coupling case extremely well, but it is also seen to describe the "normal" regime (of electronic transition probabilities greater than or similar to 0.1) even more accurately than the previous "standard" model. Published by AIP Publishing.
C1 [Miller, William H.] Univ Calif Berkeley, Dept Chem, Berkeley, CA 94720 USA.
Univ Calif Berkeley, Kenneth S Pitzer Ctr Theoret Chem, Berkeley, CA 94720 USA.
Lawrence Berkeley Natl Lab, Div Chem Sci, Berkeley, CA 94720 USA.
RP Miller, WH (reprint author), Univ Calif Berkeley, Dept Chem, Berkeley, CA 94720 USA.
EM StephenJCotton47@gmail.com; MillerWH@berkeley.edu
FU National Science Foundation [CHE-1464647]; Office of Science, Office of
Basic Energy Sciences, Chemical Sciences, Geosciences, and Biosciences
Division, U.S. Department of Energy [DE-AC02-05CH11231]; Office of
Science of the U.S. Department of Energy [DE-AC02-05CH11231]
FX This work was supported by the National Science Foundation under Grant
No. CHE-1464647 and by the Director, Office of Science, Office of Basic
Energy Sciences, Chemical Sciences, Geosciences, and Biosciences
Division, U.S. Department of Energy under Contract No.
DE-AC02-05CH11231.; In addition, this research utilized computation
resources provided by the National Energy Research Scientific Computing
Center (NERSC), which is supported by the Office of Science of the U.S.
Department of Energy under Contract No. DE-AC02-05CH11231.
NR 23
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Z9 1
U1 4
U2 4
PU AMER INST PHYSICS
PI MELVILLE
PA 1305 WALT WHITMAN RD, STE 300, MELVILLE, NY 11747-4501 USA
SN 0021-9606
EI 1089-7690
J9 J CHEM PHYS
JI J. Chem. Phys.
PD OCT 14
PY 2016
VL 145
IS 14
AR 144108
DI 10.1063/1.4963914
PG 16
WC Chemistry, Physical; Physics, Atomic, Molecular & Chemical
SC Chemistry; Physics
GA EA3VL
UT WOS:000386535900012
PM 27782507
ER
PT J
AU Grest, GS
AF Grest, Gary S.
TI Communication: Polymer entanglement dynamics: Role of attractive
interactions
SO JOURNAL OF CHEMICAL PHYSICS
LA English
DT Article
ID GLASS-TRANSITION TEMPERATURE; MOLECULAR-DYNAMICS; VISCOELASTIC
PROPERTIES; MELTS; CHAIN; RELAXATION; SIMULATION; REPTATION; LIQUIDS;
POLYETHYLENE
AB The coupled dynamics of entangled polymers, which span broad time and length scales, govern their unique viscoelastic properties. To follow chain mobility by numerical simulations from the intermediate Rouse and reptation regimes to the late time diffusive regime, highly coarse grained models with purely repulsive interactions between monomers are widely used since they are computationally the most efficient. Here using large scale molecular dynamics simulations, the effect of including the attractive interaction between monomers on the dynamics of entangled polymer melts is explored for the first time over a wide temperature range. Attractive interactions have little effect on the local packing for all temperatures T and on the chain mobility for T higher than about twice the glass transition T-g. These results, across a broad range of molecular weight, show that to study the dynamics of entangled polymer melts, the interactions can be treated as pure repulsive, confirming a posteriori the validity of previous studies and opening the way to new large scale numerical simulations. Published by AIP Publishing.
C1 [Grest, Gary S.] Sandia Natl Labs, POB 5800, Albuquerque, NM 87185 USA.
RP Grest, GS (reprint author), Sandia Natl Labs, POB 5800, Albuquerque, NM 87185 USA.
EM gsgrest@sandia.gov
FU Sandia Laboratory Directed Research and Development Program; U.S.
Department of Energy [DEAC04-94AL85000]
FX I thank Kurt Kremer, Dvora Perahia, and Mark J. Stevens for helpful
discussions. This work was supported by the Sandia Laboratory Directed
Research and Development Program. This work was performed at the Center
for Integrated Nanotechnologies, a U.S. Department of Energy, Office of
Basic Energy Sciences user facility. Sandia National Laboratories is a
multiprogram laboratory managed and operated by Sandia Corporation, a
Lockheed-Martin Company, for the U.S. Department of Energy under
Contract No. DEAC04-94AL85000.
NR 36
TC 3
Z9 3
U1 12
U2 12
PU AMER INST PHYSICS
PI MELVILLE
PA 1305 WALT WHITMAN RD, STE 300, MELVILLE, NY 11747-4501 USA
SN 0021-9606
EI 1089-7690
J9 J CHEM PHYS
JI J. Chem. Phys.
PD OCT 14
PY 2016
VL 145
IS 14
AR 141101
DI 10.1063/1.4964617
PG 4
WC Chemistry, Physical; Physics, Atomic, Molecular & Chemical
SC Chemistry; Physics
GA EA3VL
UT WOS:000386535900002
PM 27782501
ER
PT J
AU Twagirayezu, S
Hall, GE
Sears, TJ
AF Twagirayezu, Sylvestre
Hall, Gregory E.
Sears, Trevor J.
TI Quadrupole splittings in the near-infrared spectrum of (NH3)-N-14
SO JOURNAL OF CHEMICAL PHYSICS
LA English
DT Article
ID HOLLOW-CORE FIBER; HYPERFINE STRUCTURE; BAND SYSTEM; AMMONIA;
SPECTROSCOPY; ABSORPTION; ASSIGNMENTS; NU(1); NH3
AB Sub-Doppler, saturation dip, spectra of lines in the v(1) + v(3), v(1) + 2v(4), and v(3) + 2v(4) bands of (NH3)-N-14 have been measured by frequency comb-referenced diode laser absorption spectroscopy. The observed spectral line widths are dominated by transit time broadening and show resolved or partially-resolved hyperfine splittings that are primarily determined by the N-14 quadrupole coupling. Modeling of the observed line shapes based on the known hyperfine level structure of the ground state of the molecule shows that, in nearly all cases, the excited state level has hyperfine splittings similar to the same rotational level in the ground state. The data provide accurate frequencies for the line positions and easily separate lines overlapped in Doppler-limited spectra. The observed hyperfine splittings can be used to make and confirm rotational assignments and ground state combination differences obtained from the measured frequencies are comparable in accuracy to those obtained from conventional microwave spectroscopy. Several of the measured transitions do not show the quadrupole hyperfine splittings expected based on their existing rotational assignments. Either the assignments are incorrect or the upper levels involved are perturbed in a way that affects the nuclear hyperfine structure. Published by AIP Publishing.
C1 [Twagirayezu, Sylvestre; Hall, Gregory E.; Sears, Trevor J.] Brookhaven Natl Lab, Div Chem, Dept Energy & Photon Sci, Upton, NY 11973 USA.
[Sears, Trevor J.] SUNY Stony Brook, Dept Chem, Stony Brook, NY 11794 USA.
[Twagirayezu, Sylvestre] Lamar Univ, Dept Chem & Biochem, Beaumont, TX 77710 USA.
RP Twagirayezu, S (reprint author), Brookhaven Natl Lab, Div Chem, Dept Energy & Photon Sci, Upton, NY 11973 USA.; Twagirayezu, S (reprint author), Lamar Univ, Dept Chem & Biochem, Beaumont, TX 77710 USA.
EM stwagirayezu@lamar.edu; gehall@bnl.gov; sears@bnl.gov
OI Sears, Trevor/0000-0002-5559-0154; Hall, Gregory/0000-0002-8534-9783
FU U.S. Department of Energy, Office of Science [DE-SC0012704]; U.S.
Department of Energy, Office of Science by its Division of Chemical
Sciences, Geosciences and Biosciences within the Office of Basic Energy
Sciences
FX Work at Brookhaven National Laboratory was carried out under Contract
No. DE-SC0012704 with the U.S. Department of Energy, Office of Science,
and supported by its Division of Chemical Sciences, Geosciences and
Biosciences within the Office of Basic Energy Sciences.
NR 24
TC 0
Z9 0
U1 2
U2 2
PU AMER INST PHYSICS
PI MELVILLE
PA 1305 WALT WHITMAN RD, STE 300, MELVILLE, NY 11747-4501 USA
SN 0021-9606
EI 1089-7690
J9 J CHEM PHYS
JI J. Chem. Phys.
PD OCT 14
PY 2016
VL 145
IS 14
AR 144302
DI 10.1063/1.4964484
PG 8
WC Chemistry, Physical; Physics, Atomic, Molecular & Chemical
SC Chemistry; Physics
GA EA3VL
UT WOS:000386535900015
PM 27782514
ER
PT J
AU Korhonen, LC
DeGroote, NP
Shouse, RL
Valleroy, LA
Prejean, J
Bradley, H
AF Korhonen, Lauren C.
DeGroote, Nicholas P.
Shouse, R. Luke
Valleroy, Linda A.
Prejean, Joseph
Bradley, Heather
TI Unmet Needs for Ancillary Services Among Hispanics/Latinos Receiving HIV
Medical Care - United States, 2013-2014
SO MMWR-MORBIDITY AND MORTALITY WEEKLY REPORT
LA English
DT Article
C1 [Korhonen, Lauren C.; DeGroote, Nicholas P.; Shouse, R. Luke; Valleroy, Linda A.; Prejean, Joseph; Bradley, Heather] CDC, Div HIV AIDS Prevent, Natl Ctr HIV AIDS Viral Hepatitis STD & TB Preven, Atlanta, GA 30333 USA.
[Korhonen, Lauren C.; DeGroote, Nicholas P.] Oak Ridge Inst Sci & Educ, Oak Ridge, TN 37830 USA.
RP Korhonen, LC (reprint author), CDC, Div HIV AIDS Prevent, Natl Ctr HIV AIDS Viral Hepatitis STD & TB Preven, Atlanta, GA 30333 USA.; Korhonen, LC (reprint author), Oak Ridge Inst Sci & Educ, Oak Ridge, TN 37830 USA.
EM xgc9@cdc.gov
NR 10
TC 0
Z9 0
U1 0
U2 0
PU CENTERS DISEASE CONTROL
PI ATLANTA
PA 1600 CLIFTON RD, ATLANTA, GA 30333 USA
SN 0149-2195
EI 1545-861X
J9 MMWR-MORBID MORTAL W
JI MMWR-Morb. Mortal. Wkly. Rep.
PD OCT 14
PY 2016
VL 65
IS 40
BP 1104
EP 1107
PG 4
WC Public, Environmental & Occupational Health
SC Public, Environmental & Occupational Health
GA EA1AM
UT WOS:000386320700003
PM 27736837
ER
PT J
AU Liu, JM
Lin, P
Laskin, A
Laskin, J
Kathmann, SM
Wise, M
Caylor, R
Imholt, F
Selimovic, V
Shilling, JE
AF Liu, Jiumeng
Lin, Peng
Laskin, Alexander
Laskin, Julia
Kathmann, Shawn M.
Wise, Matthew
Caylor, Ryan
Imholt, Felisha
Selimovic, Vanessa
Shilling, John E.
TI Optical properties and aging of light-absorbing secondary organic
aerosol
SO ATMOSPHERIC CHEMISTRY AND PHYSICS
LA English
DT Article
ID HUMIC-LIKE SUBSTANCES; SOUTHEASTERN UNITED-STATES; BIOMASS BURNING
PARTICLES; BROWN CARBON CHROMOPHORES; COMPLEX REFRACTIVE-INDEX;
ATMOSPHERIC AEROSOLS; AMMONIUM-SULFATE; SOLAR-RADIATION; ANTHROPOGENIC
PRECURSORS; CONTINENTAL TROPOSPHERE
AB The light-absorbing organic aerosol (OA) commonly referred to as "brown carbon" (BrC) has attracted considerable attention in recent years because of its potential to affect atmospheric radiation balance, especially in the ultraviolet region and thus impact photochemical processes. A growing amount of data has indicated that BrC is prevalent in the atmosphere, which has motivated numerous laboratory and field studies; however, our understanding of the relationship between the chemical composition and optical properties of BrC remains limited. We conducted chamber experiments to investigate the effect of various volatile organic carbon (VOC) precursors, NOx concentrations, photolysis time, and relative humidity (RH) on the light absorption of selected secondary organic aerosols (SOA). Light absorption of chamber-generated SOA samples, especially aromatic SOA, was found to increase with NOx concentration, at moderate RH, and for the shortest photolysis aging times. The highest mass absorption coefficient (MAC) value is observed from toluene SOA products formed under high-NOx conditions at moderate RH, in which nitro-aromatics were previously identified as the major light-absorbing compounds. BrC light absorption is observed to decrease with photolysis time, correlated with a decline of the organic nitrate fraction of SOA. SOA formed from mixtures of aromatics and isoprene absorb less visible (Vis) and ultraviolet (UV) light than SOA formed from aromatic precursors alone on a mass basis. However, the mixed SOA absorption was underestimated when optical properties were predicted using a two-product SOA formation model, as done in many current climate models. Further investigation, including analysis on detailed mechanisms, are required to explain the discrepancy.
C1 [Liu, Jiumeng; Shilling, John E.] Pacific Northwest Natl Lab, Atmospher Sci & Global Change Div, Richland, WA 99354 USA.
[Lin, Peng; Laskin, Alexander] Pacific Northwest Natl Lab, Environm Mol Sci Lab, Richland, WA USA.
[Laskin, Julia; Kathmann, Shawn M.] Pacific Northwest Natl Lab, Phys Sci Div, Richland, WA USA.
[Wise, Matthew; Caylor, Ryan; Imholt, Felisha; Selimovic, Vanessa] Concordia Univ, Math & Sci Dept, Portland, OR USA.
[Selimovic, Vanessa] Univ Montana, Dept Chem, Missoula, MT 59812 USA.
RP Shilling, JE (reprint author), Pacific Northwest Natl Lab, Atmospher Sci & Global Change Div, Richland, WA 99354 USA.
EM john.shilling@pnnl.gov
RI Laskin, Alexander/I-2574-2012; Laskin, Julia/H-9974-2012; Lin,
Peng/G-4867-2016; Liu, Jiumeng/K-2024-2012
OI Laskin, Alexander/0000-0002-7836-8417; Laskin,
Julia/0000-0002-4533-9644; Lin, Peng/0000-0002-3567-7017; Liu,
Jiumeng/0000-0001-7238-593X
FU Laboratory Directed Research and Development funds of Pacific Northwest
National Laboratory (PNNL); DOE's Office of Biological and Environmental
Research; US Department of Energy by Battelle Memorial Institute
[DE-AC06-76RLO 1830]
FX Authors acknowledge support by the Laboratory Directed Research and
Development funds of Pacific Northwest National Laboratory (PNNL). A
portion of this study was performed at the William R. Wiley
Environmental Molecular Sciences Laboratory, a national scientific user
facility sponsored by the DOE's Office of Biological and Environmental
Research and located at PNNL. PNNL is operated for the US Department of
Energy by Battelle Memorial Institute under contract no. DE-AC06-76RLO
1830.
NR 92
TC 0
Z9 0
U1 45
U2 45
PU COPERNICUS GESELLSCHAFT MBH
PI GOTTINGEN
PA BAHNHOFSALLEE 1E, GOTTINGEN, 37081, GERMANY
SN 1680-7316
EI 1680-7324
J9 ATMOS CHEM PHYS
JI Atmos. Chem. Phys.
PD OCT 14
PY 2016
VL 16
IS 19
BP 12815
EP 12827
DI 10.5194/acp-16-12815-2016
PG 13
WC Meteorology & Atmospheric Sciences
SC Meteorology & Atmospheric Sciences
GA DY8TL
UT WOS:000385403800002
ER
PT J
AU Hazra, J
Kendrick, BK
Balakrishnan, N
AF Hazra, Jisha
Kendrick, Brian K.
Balakrishnan, N.
TI Geometric phase effects in ultracold hydrogen exchange reaction
SO JOURNAL OF PHYSICS B-ATOMIC MOLECULAR AND OPTICAL PHYSICS
LA English
DT Article
DE geometric phase effect; quantum reaction dynamics; molecular collisions;
ultracold chemistry
ID STATE TRANSITION-PROBABILITIES; SIMPLEST CHEMICAL-REACTION;
POTENTIAL-ENERGY SURFACE; COOLED COPPER TRIMER; CONICAL INTERSECTION;
SCATTERING CALCULATIONS; COLLISION ENERGIES; MOLECULAR-SYSTEMS;
IDENTICAL NUCLEI; H+O-2 SCATTERING
AB The role of the geometric phase effect on chemical reaction dynamics is explored by examining the hydrogen exchange process in the fundamental H+HD reaction. Results are presented for vibrationally excited HD molecules in the v = 4 vibrational level and for collision energies ranging from 1 mu K to 100 K. It is found that, for collision energies below 3 K, inclusion of the geometric phase leads to dramatic enhancement or suppression of the reaction rates depending on the final quantum state of the HD molecule. The effect was found to be the most prominent for rotationally resolved integral and differential cross sections but it persists to a lesser extent in the vibrationally resolved and total reaction rate coefficients. However, no significant GP effect is present in the reactive channel leading to the D+H-2 product or in the D+H-2(v = 4, j = 0) -> HD+H reaction. A simple interference mechanism involving inelastic (nonreactive) and exchange scattering amplitudes is invoked to account for the observed GP effects. The computed results also reveal a shape resonance in the H+HD reaction near 1 K and the GP effect is found to influence the magnitude of the resonant part of the cross section. Experimental detection of the resonance may allow a sensitive probe of the GP effect in the H+HD reaction.
C1 [Hazra, Jisha; Balakrishnan, N.] Univ Nevada, Dept Chem, Las Vegas, NV 89154 USA.
[Kendrick, Brian K.] Los Alamos Natl Lab, Div Theoret, T-1,MS B221, Los Alamos, NM 87545 USA.
RP Balakrishnan, N (reprint author), Univ Nevada, Dept Chem, Las Vegas, NV 89154 USA.
EM naduvala@unlv.nevada.edu
FU US Department of Energy under Project of the Laboratory Directed
Research and Development Program at Los Alamos National Laboratory
[20140309ER]; National Security Administration of the US Department of
Energy [DE-AC52-06NA25396]; Army Research Office, MURI grant
[W911NF-12-1-0476]; National Science Foundation [PHY-1505557]
FX BKK acknowledges that part of this work was done under the auspices of
the US Department of Energy under Project No. 20140309ER of the
Laboratory Directed Research and Development Program at Los Alamos
National Laboratory. Los Alamos National Laboratory is operated by Los
Alamos National Security, LLC, for the National Security Administration
of the US Department of Energy under contract DE-AC52-06NA25396. The
UNLV team acknowledges support from the Army Research Office, MURI grant
No. W911NF-12-1-0476 and the National Science Foundation, grant No.
PHY-1505557.
NR 77
TC 3
Z9 3
U1 4
U2 4
PU IOP PUBLISHING LTD
PI BRISTOL
PA TEMPLE CIRCUS, TEMPLE WAY, BRISTOL BS1 6BE, ENGLAND
SN 0953-4075
EI 1361-6455
J9 J PHYS B-AT MOL OPT
JI J. Phys. B-At. Mol. Opt. Phys.
PD OCT 14
PY 2016
VL 49
IS 19
AR 194004
DI 10.1088/0953-4075/49/19/194004
PG 14
WC Optics; Physics, Atomic, Molecular & Chemical
SC Optics; Physics
GA DY9BI
UT WOS:000385426800004
ER
PT J
AU Li, Y
Pindzola, MS
Colgan, J
AF Li, Y.
Pindzola, M. S.
Colgan, J.
TI Double photoionization of helium from the 1s2p P-3 excited state
SO JOURNAL OF PHYSICS B-ATOMIC MOLECULAR AND OPTICAL PHYSICS
LA English
DT Article
DE photoionization; cross sections; total and differential
ID DOUBLE-IONIZATION; R-MATRIX; SINGLE
AB Time-dependent close-coupling (TDCC) calculations are carried out for the double photoionization of Helium in the 1s2p P-3 excited state. TDCC l(1)l(2)L results are presented for the total and energy differential cross sections for the 1s2p P-3 term. TDCC l(1)j(1)l(2)j(2)J results are presented for the total and energy differential cross sections for the 1s2p P-3(0,1,2) levels. Differences found between the level resolved double photoionization cross sections are due to varying degrees of continuum correlation found in the outgoing two electrons.
C1 [Li, Y.; Pindzola, M. S.] Auburn Univ, Dept Phys, Auburn, AL 36849 USA.
[Colgan, J.] Los Alamos Natl Lab, Div Theoret, Los Alamos, NM USA.
RP Li, Y (reprint author), Auburn Univ, Dept Phys, Auburn, AL 36849 USA.
EM yzl006@auburn.edu
FU US National Science Foundation; US Department of Energy
FX This work was supported in part by grants from the US National Science
Foundation and the US Department of Energy. Computational work was
carried out at the National Energy Research Scientific Computing Center
in Oakland, California, and the High Performance Computing Center in
Stuttgart, Germany.
NR 11
TC 0
Z9 0
U1 4
U2 4
PU IOP PUBLISHING LTD
PI BRISTOL
PA TEMPLE CIRCUS, TEMPLE WAY, BRISTOL BS1 6BE, ENGLAND
SN 0953-4075
EI 1361-6455
J9 J PHYS B-AT MOL OPT
JI J. Phys. B-At. Mol. Opt. Phys.
PD OCT 14
PY 2016
VL 49
IS 19
AR 195205
DI 10.1088/0953-4075/49/19/195205
PG 8
WC Optics; Physics, Atomic, Molecular & Chemical
SC Optics; Physics
GA DY9BK
UT WOS:000385427000005
ER
PT J
AU Nixon, KL
Murray, AJ
Chaluvadi, H
Ning, CG
Colgan, J
Madison, DH
AF Nixon, Kate L.
Murray, Andrew J.
Chaluvadi, H.
Ning, C. G.
Colgan, James
Madison, Don H.
TI Sulphur hexaflouride: low energy (e,2e) experiments and molecular
three-body distorted wave theory
SO JOURNAL OF PHYSICS B-ATOMIC MOLECULAR AND OPTICAL PHYSICS
LA English
DT Article
DE (e,2e) spectroscopy; sulphur hexaflouride; proper average over molecular
orientations; molecular three-body distorted wave
ID CROSS-SECTIONS; SF6
AB Experimental and theoretical triple differential ionisation cross-sections (TDCSs) are presented for the highest occupied molecular orbital of sulphur hexafluoride. These measurements were performed in the low energy regime, with outgoing electron energies ranging from 5 to 40 eV in a coplanar geometry, and with energies of 10 and 20 eV in a perpendicular geometry. Complementary theoretical predictions of the TDCS were calculated using the molecular three-body distorted wave formalism. Calculations were performed using a proper average over molecular orientations as well as the orientation-averaged molecular orbital approximation. This more sophisticated model was found to be in closer agreement with the experimental data, however neither model accurately predicts the TDCS over all geometries and energies.
C1 [Nixon, Kate L.; Murray, Andrew J.] Univ Manchester, Sch Phys & Astron, Photon Sci Inst, Manchester M13 9PL, Lancs, England.
[Nixon, Kate L.] Wolverhampton Univ, Sch Biol Chem & Forens Sci, Wolverhampton WV1 1LY, W Midlands, England.
[Chaluvadi, H.; Madison, Don H.] Missouri Univ Sci & Technol, Dept Phys, Rolla, MO 65409 USA.
[Ning, C. G.] Tsinghua Univ, Dept Phys, State Key Lab Low Dimens Quantum Phys, Beijing 100084, Peoples R China.
[Colgan, James] Los Alamos Natl Lab, Div Theoret, Los Alamos, NM 87545 USA.
RP Nixon, KL (reprint author), Univ Manchester, Sch Phys & Astron, Photon Sci Inst, Manchester M13 9PL, Lancs, England.; Nixon, KL (reprint author), Wolverhampton Univ, Sch Biol Chem & Forens Sci, Wolverhampton WV1 1LY, W Midlands, England.
EM kate.nixon@wlv.ac.uk
FU European commission; US National Science Foundation [PHY-1505819];
National Natural Science Foundation of China [11174175]; Texas Advanced
Computing Center [TG-MCA07S029]; National Nuclear Security
Administration of the US Department of Energy [DE-AC5206NA25396]
FX KLN would like to thank the European commission for a Marie Curie
International Incoming Fellowship at the University of Manchester. We
would like to thank the technicians in the Schuster laboratory for
providing excellent support for the experimental apparatus. This work
was partly supported by the US National Science Foundation under Grant.
No. PHY-1505819 and by the National Natural Science Foundation of China
under Grants No. 11174175. Computational work was performed with
Institutional Computing resources made available through the Los Alamos
National Laboratory and XSEDE resources provided by the Texas Advanced
Computing Center (Grant No. TG-MCA07S029). The Los Alamos National
Laboratory is operated by Los Alamos National Security, LLC, for the
National Nuclear Security Administration of the US Department of Energy
under Contract No. DE-AC5206NA25396.
NR 29
TC 0
Z9 0
U1 6
U2 6
PU IOP PUBLISHING LTD
PI BRISTOL
PA TEMPLE CIRCUS, TEMPLE WAY, BRISTOL BS1 6BE, ENGLAND
SN 0953-4075
EI 1361-6455
J9 J PHYS B-AT MOL OPT
JI J. Phys. B-At. Mol. Opt. Phys.
PD OCT 14
PY 2016
VL 49
IS 19
AR 195203
DI 10.1088/0953-4075/49/19/195203
PG 8
WC Optics; Physics, Atomic, Molecular & Chemical
SC Optics; Physics
GA DY9BK
UT WOS:000385427000003
ER
PT J
AU Bagnoud, A
Chourey, K
Hettich, RL
de Bruijn, I
Andersson, AF
Leupin, OX
Schwyn, B
Bernier-Latmani, R
AF Bagnoud, Alexandre
Chourey, Karuna
Hettich, Robert L.
de Bruijn, Ino
Andersson, Anders F.
Leupin, Olivier X.
Schwyn, Bernhard
Bernier-Latmani, Rizlan
TI Reconstructing a hydrogen-driven microbial metabolic network in Opalinus
Clay rock
SO NATURE COMMUNICATIONS
LA English
DT Article
ID FENNOSCANDIAN SHIELD; DEEP; BIOSPHERE; WATER; SWITZERLAND; ECOSYSTEMS;
BACTERIA; AQUIFERS; REVEALS; LIFE
AB The Opalinus Clay formation will host geological nuclear waste repositories in Switzerland. It is expected that gas pressure will build-up due to hydrogen production from steel corrosion, jeopardizing the integrity of the engineered barriers. In an in situ experiment located in the Mont Terri Underground Rock Laboratory, we demonstrate that hydrogen is consumed by microorganisms, fuelling a microbial community. Metagenomic binning and metaproteomic analysis of this deep subsurface community reveals a carbon cycle driven by autotrophic hydrogen oxidizers belonging to novel genera. Necromass is then processed by fermenters, followed by complete oxidation to carbon dioxide by heterotrophic sulfate-reducing bacteria, which closes the cycle. This microbial metabolic web can be integrated in the design of geological repositories to reduce pressure build-up. This study shows that Opalinus Clay harbours the potential for chemolithoautotrophic-based system, and provides a model of microbial carbon cycle in deep subsurface environments where hydrogen and sulfate are present.
C1 [Bagnoud, Alexandre; Bernier-Latmani, Rizlan] Ecole Polytech Fed Lausanne, Environm Microbiol Lab, Stn 6, CH-1015 Lausanne, Switzerland.
[Chourey, Karuna; Hettich, Robert L.] Oak Ridge Natl Lab, Div Chem Sci, Oak Ridge, TN 37831 USA.
[de Bruijn, Ino] Bioinformat Infrastruct Life Sci, S-17165 Stockholm, Sweden.
[de Bruijn, Ino; Andersson, Anders F.] KTH Royal Inst Technol, Sci Life Lab, Sch Biotechnol, Div Gene Technol, S-17165 Stockholm, Sweden.
[Leupin, Olivier X.; Schwyn, Bernhard] Nagra, CH-5430 Wettingen, Switzerland.
[Bagnoud, Alexandre] Ecole Polytech Fed Lausanne, Stream Biofilm & Ecol Res Lab, Stn 2, CH-1015 Lausanne, Switzerland.
RP Bernier-Latmani, R (reprint author), Ecole Polytech Fed Lausanne, Environm Microbiol Lab, Stn 6, CH-1015 Lausanne, Switzerland.
EM rizlan.bernier-latmani@epfl.ch
RI Bernier-Latmani, Rizlan/E-4398-2011;
OI Bernier-Latmani, Rizlan/0000-0001-6547-722X; de Bruijn,
Ino/0000-0001-5427-4750; Andersson, Anders/0000-0002-3627-6899
FU Office of Science of the U.S. Department of Energy [DE-AC02-05CH11231];
U.S. Department of Energy's Genomic Science Program; Swedish Research
Council VR [2011-5689]; [CSP 1505]
FX We thank Manon Frutschi for her invaluable help during sampling. We are
grateful to the Swisstopo team of the Mont Terri Underground Rock
Laboratory that provides optimal conditions for scientific research,
particularly Thierry Theurillat and Nicola Kern. We thank also Yanick
Lettry, Thomas Fierz and Herwig Mueller for their help in designing and
running the system. The work conducted by the U.S. Department of Energy
Joint Genome Institute (JGI) is supported by the Office of Science of
the U.S. Department of Energy under Contract No. DE-AC02-05CH11231. K.C
and R.L.H. acknowledge support from U.S. Department of Energy's Genomic
Science Program. JGI is acknowledged for providing resources for the
sequencing analysis through the grant CSP 1505 to R.B.-L. A.F.A. is
supported by a grant from the Swedish Research Council VR (grant
2011-5689). Computations were performed on resources provided by the
Swedish National Infrastructure for Computing (SNIC).
NR 46
TC 1
Z9 1
U1 22
U2 22
PU NATURE PUBLISHING GROUP
PI LONDON
PA MACMILLAN BUILDING, 4 CRINAN ST, LONDON N1 9XW, ENGLAND
SN 2041-1723
J9 NAT COMMUN
JI Nat. Commun.
PD OCT 14
PY 2016
VL 7
AR 12770
DI 10.1038/ncomms12770
PG 10
WC Multidisciplinary Sciences
SC Science & Technology - Other Topics
GA DZ0QV
UT WOS:000385545700001
PM 27739431
ER
PT J
AU Jozwiak, C
Sobota, JA
Gotlieb, K
Kemper, AF
Rotundu, CR
Birgeneau, RJ
Hussain, Z
Lee, DH
Shen, ZX
Lanzara, A
AF Jozwiak, Chris
Sobota, Jonathan A.
Gotlieb, Kenneth
Kemper, Alexander F.
Rotundu, Costel R.
Birgeneau, Robert J.
Hussain, Zahid
Lee, Dung-Hai
Shen, Zhi-Xun
Lanzara, Alessandra
TI Spin-polarized surface resonances accompanying topological surface state
formation
SO NATURE COMMUNICATIONS
LA English
DT Article
ID INITIO MOLECULAR-DYNAMICS; TOTAL-ENERGY CALCULATIONS; AUGMENTED-WAVE
METHOD; SINGLE DIRAC CONE; PHASE-TRANSITION; BASIS-SET; INSULATORS;
BI2TE3; METALS
AB Topological insulators host spin-polarized surface states born out of the energetic inversion of bulk bands driven by the spin-orbit interaction. Here we discover previously unidentified consequences of band-inversion on the surface electronic structure of the topological insulator Bi2Se3. By performing simultaneous spin, time, and angle-resolved photoemission spectroscopy, we map the spin-polarized unoccupied electronic structure and identify a surface resonance which is distinct from the topological surface state, yet shares a similar spin-orbital texture with opposite orientation. Its momentum dependence and spin texture imply an intimate connection with the topological surface state. Calculations show these two distinct states can emerge from trivial Rashba-like states that change topology through the spin-orbit-induced band inversion. This work thus provides a compelling view of the coevolution of surface states through a topological phase transition, enabled by the unique capability of directly measuring the spin-polarized unoccupied band structure.
C1 [Jozwiak, Chris; Sobota, Jonathan A.; Hussain, Zahid] Lawrence Berkeley Natl Lab, Adv Light Source, Berkeley, CA 94720 USA.
[Sobota, Jonathan A.; Rotundu, Costel R.; Shen, Zhi-Xun] SLAC Natl Accelerator Lab, Stanford Inst Mat & Energy Sci, 2575 Sand Hill Rd, Menlo Pk, CA 94025 USA.
[Sobota, Jonathan A.; Shen, Zhi-Xun] Stanford Univ, Geballe Lab Adv Mat, Dept Phys, Stanford, CA 94305 USA.
[Sobota, Jonathan A.; Shen, Zhi-Xun] Stanford Univ, Geballe Lab Adv Mat, Dept Appl Phys, Stanford, CA 94305 USA.
[Gotlieb, Kenneth] Univ Calif Berkeley, Grad Grp Appl Sci & Technol, Berkeley, CA 94720 USA.
[Kemper, Alexander F.] North Carolina State Univ, Dept Phys, Raleigh, NC 27695 USA.
[Kemper, Alexander F.] Lawrence Berkeley Natl Lab, Computat Res Div, Berkeley, CA 94720 USA.
[Birgeneau, Robert J.; Lee, Dung-Hai; Lanzara, Alessandra] Lawrence Berkeley Natl Lab, Div Mat Sci, Berkeley, CA 94720 USA.
[Birgeneau, Robert J.; Lee, Dung-Hai; Lanzara, Alessandra] Univ Calif Berkeley, Dept Phys, Berkeley, CA 94720 USA.
[Birgeneau, Robert J.] Univ Calif Berkeley, Dept Mat Sci & Engn, Berkeley, CA 94720 USA.
RP Jozwiak, C (reprint author), Lawrence Berkeley Natl Lab, Adv Light Source, Berkeley, CA 94720 USA.; Lanzara, A (reprint author), Lawrence Berkeley Natl Lab, Div Mat Sci, Berkeley, CA 94720 USA.; Lanzara, A (reprint author), Univ Calif Berkeley, Dept Phys, Berkeley, CA 94720 USA.
EM CMJozwiak@lbl.gov; ALanzara@lbl.gov
FU Office of Science, Office of Basic Energy Sciences, Materials Sciences
and Engineering Division, of the U.S. Department of Energy
[DE-AC02-05CH11231, DE-AC02-76SF00515]; Ultrafast Materials Science
Program [KC2203]; Advanced Light Source; Office of Science, Office of
Basic Energy Sciences, of the U.S. Department of Energy
[DE-AC02-05CH11231]; Gordon and Betty Moore Foundation's EPiQS
Initiative [GBMF4546]; Quantum Materials Program [KC2202]; Laboratory
Directed Research and Development Program of Lawrence Berkeley National
Laboratory under U.S. Department of Energy [DE-AC02-05CH11231]
FX We thank A. Bostwick for significant help with software development, and
P.S. Kirchmann and S.-L. Yang for meaningful discussions. This work was
mainly supported by the Director, Office of Science, Office of Basic
Energy Sciences, Materials Sciences and Engineering Division, of the
U.S. Department of Energy, under Contract No. DE-AC02-05CH11231, as part
of the Ultrafast Materials Science Program (KC2203). C.J. and Z.H. were
supported by the Advanced Light Source, which is supported by the
Director, Office of Science, Office of Basic Energy Sciences, of the
U.S. Department of Energy under Contract No. DE-AC02-05CH11231. J.A.S.
and Z.-X.S. were primarily supported by the Director, Office of Science,
Office of Basic Energy Sciences, Materials Sciences and Engineering
Division, of the U.S. Department of Energy, under Contract No.
DE-AC02-76SF00515, and in part by the Gordon and Betty Moore
Foundation's EPiQS Initiative through Grant GBMF4546. Sample growth and
theoretical work were supported by the Director, Office of Science,
Office of Basic Energy Sciences, Materials Sciences and Engineering
Division, of the U.S. Department of Energy, under Contract No.
DE-AC02-05CH11231 as part of the Quantum Materials Program (KC2202).
A.F.K. was in part supported by the Laboratory Directed Research and
Development Program of Lawrence Berkeley National Laboratory under U.S.
Department of Energy Contract No. DE-AC02-05CH11231.
NR 44
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U1 21
U2 21
PU NATURE PUBLISHING GROUP
PI LONDON
PA MACMILLAN BUILDING, 4 CRINAN ST, LONDON N1 9XW, ENGLAND
SN 2041-1723
J9 NAT COMMUN
JI Nat. Commun.
PD OCT 14
PY 2016
VL 7
AR 13143
DI 10.1038/ncomms13143
PG 7
WC Multidisciplinary Sciences
SC Science & Technology - Other Topics
GA DZ0SA
UT WOS:000385548800001
PM 27739428
ER
PT J
AU Ralevic, U
Lazarevic, N
Baum, A
Eiter, HM
Hackl, R
Giraldo-Gallo, P
Fisher, IR
Petrovic, C
Gajic, R
Popovic, ZV
AF Ralevic, U.
Lazarevic, N.
Baum, A.
Eiter, H. -M.
Hackl, R.
Giraldo-Gallo, P.
Fisher, I. R.
Petrovic, C.
Gajic, R.
Popovic, Z. V.
TI Charge density wave modulation and gap measurements in CeTe3
SO PHYSICAL REVIEW B
LA English
DT Article
ID RARE-EARTH-ELEMENT; ELECTRONIC-STRUCTURE; SQUARE NETS; RETE3 RE;
SUPERCONDUCTORS; TELLURIUM; NBSE2; ORDER
AB We present a study of charge density wave (CDW) ordering in CeTe3 at room temperature using a scanning tunneling microscope and Raman spectroscopy. Two characteristic CDW ordering wave vectors obtained from the Fourier analysis are assessed to be |c* - q| = 4.19 nm(-1) and |q| = 10.26 nm(-1) where |c*| = 2 Pi/c is the reciprocal lattice vector. The scanning tunneling spectroscopy measurements, along with inelastic light ( Raman) scattering measurements, show a CDWgap Delta(max) of approximately 0.37 eV. In addition to the CDW modulation, we observe an organization of the Te sheet atoms in an array of alternating V- and N-shaped groups along the CDW modulation, as predicted in the literature.
C1 [Ralevic, U.; Lazarevic, N.; Gajic, R.; Popovic, Z. V.] Univ Belgrade, Inst Phys, Ctr Solid State Phys & New Mat, Pregrevica 118, Belgrade 11080, Serbia.
[Ralevic, U.] Univ Belgrade, Fac Elect Engn, Bulevar Kralja Aleksandra 73b, Belgrade 11120, Serbia.
[Baum, A.; Eiter, H. -M.; Hackl, R.] Bayer Akad Wissensch, Walther Meissner Inst, D-85748 Garching, Germany.
[Giraldo-Gallo, P.] Stanford Univ, Dept Phys, Stanford, CA 94305 USA.
[Fisher, I. R.] Stanford Univ, Dept Appl Phys, Stanford, CA 94305 USA.
[Giraldo-Gallo, P.; Fisher, I. R.] SLAC Natl Accelerator Lab, Stanford Inst Mat & Energy Sci, 2575 Sand Hill Rd, Menlo Pk, CA 94025 USA.
[Petrovic, C.] Brookhaven Natl Lab, Condensed Matter Phys & Mat Sci Dept, Upton, NY 11973 USA.
RP Ralevic, U (reprint author), Univ Belgrade, Inst Phys, Ctr Solid State Phys & New Mat, Pregrevica 118, Belgrade 11080, Serbia.; Ralevic, U (reprint author), Univ Belgrade, Fac Elect Engn, Bulevar Kralja Aleksandra 73b, Belgrade 11120, Serbia.
FU Serbian Ministry of Education, Science, and Technological Development
[ON171032, III45018, OI171005.]; DAAD through the bilateral project
between Serbia and Germany [56267076, 57142964]; DFG via the
Transregional Collaborative Research Center [TRR 80]; Bavarian
Californian Technology Center BaCaTeC [A5 [2012-2]]; US Department of
Energy, Office of Basic Energy Sciences, Division of Materials Sciences
and Engineering [DE-AC02-76SF00515]
FX This work was supported by the Serbian Ministry of Education, Science,
and Technological Development under Projects No. ON171032, No. III45018,
and No. OI171005. We acknowledge support by the DAAD through the
bilateral project between Serbia and Germany (Grants No. 56267076 and
No. 57142964) and the DFG via the Transregional Collaborative Research
Center TRR 80. The collaboration with Stanford University was supported
by the Bavarian Californian Technology Center BaCaTeC (Grant No. A5
[2012-2]). Work in the SIMES at Stanford University and SLAC was
supported by the US Department of Energy, Office of Basic Energy
Sciences, Division of Materials Sciences and Engineering, under Contract
No. DE-AC02-76SF00515. Part of the work was carried out at the
Brookhaven National Laboratory, which is operated for the Office of
Basic Energy Sciences, US Department of Energy, by Brookhaven Science
Associates (DE-SC0012704). We are grateful to Nenad Stojilovic for
useful discussions.
NR 37
TC 0
Z9 0
U1 13
U2 13
PU AMER PHYSICAL SOC
PI COLLEGE PK
PA ONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA
SN 2469-9950
EI 2469-9969
J9 PHYS REV B
JI Phys. Rev. B
PD OCT 14
PY 2016
VL 94
IS 16
AR 165132
DI 10.1103/PhysRevB.94.165132
PG 8
WC Physics, Condensed Matter
SC Physics
GA DZ1VF
UT WOS:000385628600007
ER
PT J
AU Rego, L
San Roman, J
Picon, A
Plaja, L
Hernandez-Garcia, C
AF Rego, Laura
San Roman, Julio
Picon, Antonio
Plaja, Luis
Hernandez-Garcia, Carlos
TI Nonperturbative Twist in the Generation of Extreme-Ultraviolet Vortex
Beams
SO PHYSICAL REVIEW LETTERS
LA English
DT Article
ID HIGH-HARMONIC-GENERATION; ORBITAL ANGULAR-MOMENTUM; 2ND-HARMONIC
GENERATION; ATTOSECOND PULSES; CYCLE REGIME; LIGHT-BEAMS; VORTICES;
PHYSICS; FIELD; POLARIZATION
AB High-order harmonic generation (HHG) has been recently proven to produce extreme-ultraviolet (XUV) vortices from the nonlinear conversion of infrared twisted beams. Previous works have demonstrated a linear scaling law of the vortex charge with the harmonic order. We demonstrate that this simple law hides an unexpectedly rich scenario for the buildup of orbital angular momentum (OAM) due to the nonperturbative behavior of HHG. The complexity of these twisted XUV beams appears only when HHG is driven by nonpure vortex modes, where the XUV OAM content is dramatically increased. We explore the underlying mechanisms for this diversity and derive a general conservation rule for the nonperturbative OAM buildup. The simple scaling found in previous works corresponds to the collapse of this scenario for the particular case of pure (single-mode) OAM driving fields.
C1 [Rego, Laura; San Roman, Julio; Plaja, Luis; Hernandez-Garcia, Carlos] Univ Salamanca, Dept Fis Aplicada, Grp Invest Aplicac Laser & Foton, E-37008 Salamanca, Spain.
[Picon, Antonio] Argonne Natl Lab, Argonne, IL 60439 USA.
RP Rego, L (reprint author), Univ Salamanca, Dept Fis Aplicada, Grp Invest Aplicac Laser & Foton, E-37008 Salamanca, Spain.
EM laura.rego@usal.es; carloshergar@usal.es
RI Hernandez-Garcia, Carlos/G-3681-2011; Plaja, Luis/K-8701-2014; San
Roman, Julio/K-7218-2012
OI Hernandez-Garcia, Carlos/0000-0002-6153-2647; Plaja,
Luis/0000-0001-8709-7295; San Roman, Julio/0000-0002-2645-7039
FU Marie Curie International Outgoing Fellowship within the EU Seventh
Framework Programme for Research and Technological Development, REA
Grant Agreement [328334]; Junta de Castilla y Leon [SA116U13, SA046U16];
Ministerio de Economia y Competitividad [FIS2013-44174-P,
FIS2016-75652-P]; U.S. Department of Energy, Office of Science, Basic
Energy Sciences, Chemical Sciences, Geosciences, and Biosciences
Division [DE-AC0-206CH11357]
FX C. H.-G. acknowledges support by a Marie Curie International Outgoing
Fellowship within the EU Seventh Framework Programme for Research and
Technological Development (2007-2013), under REA Grant Agreement No.
328334. We acknowledge support from Junta de Castilla y Leon (Projects
No. SA116U13 and No. SA046U16) and Ministerio de Economia y
Competitividad (FIS2013-44174-P, FIS2016-75652-P). A. P. acknowledges
support from the U.S. Department of Energy, Office of Science, Basic
Energy Sciences, Chemical Sciences, Geosciences, and Biosciences
Division under Contract No. DE-AC02-06CH11357.
NR 57
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U1 11
U2 11
PU AMER PHYSICAL SOC
PI COLLEGE PK
PA ONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA
SN 0031-9007
EI 1079-7114
J9 PHYS REV LETT
JI Phys. Rev. Lett.
PD OCT 14
PY 2016
VL 117
IS 16
AR 163202
DI 10.1103/PhysRevLett.117.163202
PG 6
WC Physics, Multidisciplinary
SC Physics
GA DZ1ZT
UT WOS:000385641900006
PM 27792355
ER
PT J
AU Schenke, B
Schlichting, S
Tribedy, P
Venugopalan, R
AF Schenke, Bjoern
Schlichting, Soeren
Tribedy, Prithwish
Venugopalan, Raju
TI Mass Ordering of Spectra from Fragmentation of Saturated Gluon States in
High-Multiplicity Proton-Proton Collisions
SO PHYSICAL REVIEW LETTERS
LA English
DT Article
ID P-PB COLLISIONS; LONG-RANGE; ANGULAR-CORRELATIONS; AZIMUTHAL HARMONICS;
TRANSVERSE-MOMENTUM; ION COLLISIONS; LARGE NUCLEI; PLUS; TEV; DEPENDENCE
AB The mass ordering of mean transverse momentum p(T) and of the Fourier harmonic coefficient v(2)(p(T)) of azimuthally anisotropic particle distributions in high energy hadron collisions is often interpreted as evidence for the hydrodynamic flow of the matter produced. We investigate an alternative initial state interpretation of this pattern in high-multiplicity proton-proton collisions at the LHC. The QCDYang-Mills equations describing the dynamics of saturated gluons are solved numerically with initial conditions obtained from the color-glass-condensate-based impact-parameter-dependent glasma model. The gluons are subsequently fragmented into various hadron species employing the well established Lund string fragmentation algorithm of the PYTHIA event generator. We find that this initial state approach reproduces characteristic features of bulk spectra, in particular, the particle mass dependence of p(T) and v(2)(p(T)).
C1 [Schenke, Bjoern; Schlichting, Soeren; Tribedy, Prithwish; Venugopalan, Raju] Brookhaven Natl Lab, Dept Phys, Upton, NY 11973 USA.
[Venugopalan, Raju] Heidelberg Univ, Inst Theoret Phys, Philosophenweg 16, D-69120 Heidelberg, Germany.
RP Schenke, B (reprint author), Brookhaven Natl Lab, Dept Phys, Upton, NY 11973 USA.
FU U.S. Department of Energy, Office of Science [DE-SC0012704]; Excellence
Initiative of Heidelberg University; Office of Science of the U.S.
Department of Energy [DE-AC02-05CH11231]; Brookhaven Science Associates
FX We thank Christian Bierlich, Ilkka Helenius, Wei Li, Subhash Singha, and
Takahito Todoroki for important discussions. This work is supported in
part by the U.S. Department of Energy, Office of Science, under Contract
No. DE-SC0012704. R. V. thanks the Institut fur Theoretische Physik,
Heidelberg, for their kind hospitality and the Excellence Initiative of
Heidelberg University for support. This research used resources of the
National Energy Research Scientific Computing Center, a DOE Office of
Science User Facility supported by the Office of Science of the U.S.
Department of Energy under Contract No. DE-AC02-05CH11231. S. S.
gratefully acknowledges support from the Brookhaven Science Associates.
NR 77
TC 2
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U1 0
U2 0
PU AMER PHYSICAL SOC
PI COLLEGE PK
PA ONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA
SN 0031-9007
EI 1079-7114
J9 PHYS REV LETT
JI Phys. Rev. Lett.
PD OCT 14
PY 2016
VL 117
IS 16
AR 162301
DI 10.1103/PhysRevLett.117.162301
PG 6
WC Physics, Multidisciplinary
SC Physics
GA DZ1ZT
UT WOS:000385641900002
PM 27792356
ER
PT J
AU Kim, J
Nam, H
Li, GR
Karki, AB
Wang, Z
Zhu, YM
Shih, CK
Zhang, JD
Jin, RY
Plummer, EW
AF Kim, Jisun
Nam, Hyoungdo
Li, Guorong
Karki, A. B.
Wang, Zhen
Zhu, Yimei
Shih, Chih-Kang
Zhang, Jiandi
Jin, Rongying
Plummer, E. W.
TI Interrogating the superconductor Ca-10(Pt4As8)(Fe2-xPtxAs2)(5)
Layer-by-layer
SO SCIENTIFIC REPORTS
LA English
DT Article
ID IRON; CA-10(PT4AS8)(FE2AS2)(5)
AB Ever since the discovery of high-T-c superconductivity in layered cuprates, the roles that individual layers play have been debated, due to difficulty in layer-by-layer characterization. While there is similar challenge in many Fe-based layered superconductors, the newly-discovered Ca-10(Pt4As8) (Fe2As2)(5) provides opportunities to explore superconductivity layer by layer, because it contains both superconducting building blocks (Fe2As2 layers) and intermediate Pt4As8 layers. Cleaving a single crystal under ultra-high vacuum results in multiple terminations: an ordered Pt4As8 layer, two reconstructed Ca layers on the top of a Pt4As8 layer, and disordered Ca layer on the top of Fe2As2 layer. The electronic properties of individual layers are studied using scanning tunneling microscopy/spectroscopy (STM/S), which reveals different spectra for each surface. Remarkably superconducting coherence peaks are seen only on the ordered Ca/Pt4As8 layer. Our results indicate that an ordered structure with proper charge balance is required in order to preserve superconductivity.
C1 [Kim, Jisun; Li, Guorong; Karki, A. B.; Wang, Zhen; Zhang, Jiandi; Jin, Rongying; Plummer, E. W.] Louisiana State Univ, Dept Phys & Astron, Baton Rouge, LA 70803 USA.
[Nam, Hyoungdo; Shih, Chih-Kang] Univ Texas Austin, Dept Phys, Austin, TX 78712 USA.
[Wang, Zhen; Zhu, Yimei] Brookhaven Natl Lab, Upton, NY 11973 USA.
RP Plummer, EW (reprint author), Louisiana State Univ, Dept Phys & Astron, Baton Rouge, LA 70803 USA.
EM wplummer@phys.lsu.edu
FU NSF-DMR [1504226, ONR-N00014-14-1-0330]; DOE [DE-SC0002136]; U.S.
Department of Energy, Office of Basic Energy Science [DE-AC02-98CH10886]
FX This work was supported by NSF-DMR 1504226 (J.K., G.L., A.K., R.J. and
E.W.P.), ONR-N00014-14-1-0330 (H.N. and C.K.S.), DOE DE-SC0002136 (Z.W.
and J.Z.). The STEM measurement was conducted in Brookhaven National
Laboratory which was supported by the U.S. Department of Energy, Office
of Basic Energy Science, under Contract No. DE-AC02-98CH10886 (Y.Z.).
NR 29
TC 0
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U1 7
U2 7
PU NATURE PUBLISHING GROUP
PI LONDON
PA MACMILLAN BUILDING, 4 CRINAN ST, LONDON N1 9XW, ENGLAND
SN 2045-2322
J9 SCI REP-UK
JI Sci Rep
PD OCT 14
PY 2016
VL 6
AR 35365
DI 10.1038/srep35365
PG 9
WC Multidisciplinary Sciences
SC Science & Technology - Other Topics
GA DY7JR
UT WOS:000385306100001
PM 27739517
ER
PT J
AU May, AF
Calder, S
Parker, DS
Sales, BC
McGuire, MA
AF May, Andrew F.
Calder, Stuart
Parker, David S.
Sales, Brian C.
McGuire, Michael A.
TI Competing magnetic ground states and their coupling to the crystal
lattice in CuFe2Ge2
SO SCIENTIFIC REPORTS
LA English
DT Article
ID IRON; NICKEL; ENERGY
AB Identifying and characterizing systems with coupled and competing interactions is central to the development of physical models that can accurately describe and predict emergent behavior in condensed matter systems. This work demonstrates that the metallic compound CuFe2Ge2 has competing magnetic ground states, which are shown to be strongly coupled to the lattice and easily manipulated using temperature and applied magnetic fields. Temperature-dependent magnetization M measurements reveal a ferromagnetic-like onset at 228 (1) K and a broad maximum in M near 180 K. Powder neutron diffraction confirms antiferromagnetic ordering below T-N approximate to 175 K, and an incommensurate spin density wave is observed below approximate to 125 K. Coupled with the small refined moments (0.5-1 mu B/Fe), this provides a picture of itinerant magnetism in CuFe2Ge2. The neutron diffraction data also reveal a coexistence of two magnetic phases that further highlights the near-degeneracy of various magnetic states. These results demonstrate that the ground state in CuFe2Ge2 can be easily manipulated by external forces, making it of particular interest for doping, pressure, and further theoretical studies.
C1 [May, Andrew F.; Parker, David S.; Sales, Brian C.; McGuire, Michael A.] Oak Ridge Natl Lab, Div Mat Sci & Technol, Oak Ridge, TN 37831 USA.
[Calder, Stuart] Oak Ridge Natl Lab, Quantum Condensed Matter Div, Oak Ridge, TN 37831 USA.
RP May, AF (reprint author), Oak Ridge Natl Lab, Div Mat Sci & Technol, Oak Ridge, TN 37831 USA.
EM mayaf@ornl.gov
RI McGuire, Michael/B-5453-2009; May, Andrew/E-5897-2011
OI McGuire, Michael/0000-0003-1762-9406; May, Andrew/0000-0003-0777-8539
FU U.S. Department of Energy, Office of Science, Basic Energy Sciences,
Materials Sciences and Engineering Division
FX This work was supported by the U.S. Department of Energy, Office of
Science, Basic Energy Sciences, Materials Sciences and Engineering
Division. A portion of this research used resources at the High Flux
Isotope Reactor, a DOE Office of Science User Facility operated by the
Oak Ridge National Laboratory. We thank Huibo Cao for assistance with
preliminary neutron diffraction experiments and Jiaqiang Yan for useful
discussions.
NR 17
TC 0
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U1 6
U2 6
PU NATURE PUBLISHING GROUP
PI LONDON
PA MACMILLAN BUILDING, 4 CRINAN ST, LONDON N1 9XW, ENGLAND
SN 2045-2322
J9 SCI REP-UK
JI Sci Rep
PD OCT 14
PY 2016
VL 6
AR 35325
DI 10.1038/srep35325
PG 9
WC Multidisciplinary Sciences
SC Science & Technology - Other Topics
GA DY7MV
UT WOS:000385314300002
PM 27739477
ER
PT J
AU Yu, W
Jiang, Y
Yang, J
Dun, ZL
Zhou, HD
Jiang, Z
Lu, P
Pan, W
AF Yu, W.
Jiang, Y.
Yang, J.
Dun, Z. L.
Zhou, H. D.
Jiang, Z.
Lu, P.
Pan, W.
TI Quantum Oscillations at Integer and Fractional Landau Level Indices in
Single-Crystalline ZrTe5
SO SCIENTIFIC REPORTS
LA English
DT Article
ID TOPOLOGICAL DIRAC SEMIMETAL; SURFACE-STATES; BERRYS PHASE; GRAPHENE;
MAGNETORESISTANCE; INSULATOR; HFTE5; METAL
AB A three-dimensional (3D) Dirac semimetal (DS) is an analogue of graphene, but with linear energy dispersion in all (three) momentum directions. 3D DSs have been a fertile playground in discovering novel quantum particles, for example Weyl fermions, in solid state systems. Many 3D DSs were theoretically predicted and experimentally confirmed. We report here the results in exfoliated ZrTe5 thin flakes from the studies of aberration-corrected scanning transmission electron microscopy and low temperature magneto-transport measurements. Several unique results were observed. First, a pi Berry phase was obtained from the Landau fan diagram of the Shubnikov-de Haas oscillations in the longitudinal conductivity sigma(xx). Second, the longitudinal resistivity rho(xx) shows a linear magnetic field dependence in the quantum limit regime. Most surprisingly, quantum oscillations were also observed at fractional Landau level indices N = 5/3 and 7/5, demonstrating strong electron-electron interaction effects in ZrTe5.
C1 [Yu, W.; Lu, P.; Pan, W.] Sandia Natl Labs, Albuquerque, NM 87185 USA.
[Jiang, Y.; Yang, J.; Jiang, Z.] Georgia Inst Technol, Sch Phys, Atlanta, GA 30332 USA.
[Dun, Z. L.; Zhou, H. D.] Univ Tennessee, Dept Phys & Astron, Knoxville, TN 37996 USA.
RP Yu, W (reprint author), Sandia Natl Labs, Albuquerque, NM 87185 USA.
EM wnyu@sandia.gov
RI Dun, Zhiling/F-5617-2016; Zhou, Haidong/O-4373-2016
OI Dun, Zhiling/0000-0001-6653-3051;
FU U.S. Department of Energy, Office of Science, Basic Energy Sciences,
Materials Sciences and Engineering Division; U.S. Department of Energy's
National Nuclear Security Administration [DE-AC04-94AL85000]; Department
of Energy [DE-FG02-07ER46451]; National Science Foundation [DMR-1350002]
FX This work was supported by the U.S. Department of Energy, Office of
Science, Basic Energy Sciences, Materials Sciences and Engineering
Division. Sandia National Laboratories is a multi-program laboratory
managed and operated by Sandia Corporation, a wholly owned subsidiary of
Lockheed Martin Corporation, for the U.S. Department of Energy's
National Nuclear Security Administration under contract
DE-AC04-94AL85000. Work at Georgia Institute of Technology was, in part,
supported by the Department of Energy (Grant No. DE-FG02-07ER46451).
ZrTe5 single crystal growth at University of Tennessee was
supported by the National Science Foundation (Grant No. DMR-1350002).
NR 37
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U1 32
U2 32
PU NATURE PUBLISHING GROUP
PI LONDON
PA MACMILLAN BUILDING, 4 CRINAN ST, LONDON N1 9XW, ENGLAND
SN 2045-2322
J9 SCI REP-UK
JI Sci Rep
PD OCT 14
PY 2016
VL 6
AR 35357
DI 10.1038/srep35357
PG 7
WC Multidisciplinary Sciences
SC Science & Technology - Other Topics
GA DY7JM
UT WOS:000385305600001
PM 27739474
ER
PT J
AU Howes, NUM
Lockhart, JPA
Blitz, MA
Carr, SA
Baeza-Romero, MT
Heard, DE
Shannon, RJ
Seakins, PW
Varga, T
AF Howes, Neil U. M.
Lockhart, James P. A.
Blitz, Mark A.
Carr, Scott A.
Teresa Baeza-Romero, Maria
Heard, Dwayne E.
Shannon, Robin J.
Seakins, Paul W.
Varga, T.
TI Observation of a new channel, the production of CH3, in the abstraction
reaction of OH radicals with acetaldehyde
SO PHYSICAL CHEMISTRY CHEMICAL PHYSICS
LA English
DT Article
ID RATE COEFFICIENTS; PRESSURE-DEPENDENCE; HYDROXYL RADICALS;
MASS-SPECTROMETRY; KINETICS; ACETONE; YIELDS; O-2; TEMPERATURE;
CHEMISTRY
AB Using laser flash photolysis coupled to photo-ionization time-of-flight mass spectrometry (PIMS), methyl radicals (CH3) have been detected as primary products from the reaction of OH radicals with acetaldehyde (ethanal, CH3CHO) with a yield of similar to 15% at 1-2 Torr of helium bath gas. Supporting measurements based on laser induced fluorescence studies of OH recycling in the OH/CH3CHO/O-2 system are consistent with the PIMS study. Master equation calculations suggest that the origin of the methyl radicals is from prompt dissociation of chemically activated acetyl products and hence is consistent with previous studies which have shown that abstraction, rather than addition/elimination, is the sole route for the OH + acetaldehyde reaction. However, the observation of a significant methyl product yield suggests that energy partitioning in the reaction is different from the typical early barrier mechanism where reaction exothermicity is channeled preferentially into the newly formed bond. The master equation calculations predict atmospheric yields of methyl radicals of similar to 9%. The implications of the observations in atmospheric and combustion chemistry are briefly discussed.
C1 [Howes, Neil U. M.; Lockhart, James P. A.; Carr, Scott A.; Teresa Baeza-Romero, Maria; Shannon, Robin J.; Varga, T.] Univ Leeds, Sch Chem, Leeds LS2 9JT, W Yorkshire, England.
[Blitz, Mark A.; Heard, Dwayne E.; Seakins, Paul W.] Univ Leeds, Natl Ctr Atmospher Sci, Leeds LS2 9JT, W Yorkshire, England.
[Lockhart, James P. A.] Argonne Natl Lab, 9700 S Cass Ave, Argonne, IL 60439 USA.
[Teresa Baeza-Romero, Maria] Escuela Ingn Ind Toledo, Toledo, Spain.
[Shannon, Robin J.] Univ Bristol, Bristol, Avon, England.
[Varga, T.] Eotvos Lorand Univ, Inst Chem, Budapest, Hungary.
RP Blitz, MA; Seakins, PW (reprint author), Univ Leeds, Natl Ctr Atmospher Sci, Leeds LS2 9JT, W Yorkshire, England.
EM m.blitz@leeds.ac.uk; p.w.seakins@leeds.ac.uk
RI Varga, Tamas/A-2930-2015
OI Varga, Tamas/0000-0002-6500-9546
FU NERC; EPSRC [GR/T28560/01, EP/J010871/1]
FX The authors are grateful to NERC for studentships for NUMH, and JPAL, to
EPSRC for a studentship for SAC (Grant GR/T28560/01) and support for RJS
(Grant EP/J010871/1).
NR 55
TC 0
Z9 0
U1 20
U2 20
PU ROYAL SOC CHEMISTRY
PI CAMBRIDGE
PA THOMAS GRAHAM HOUSE, SCIENCE PARK, MILTON RD, CAMBRIDGE CB4 0WF, CAMBS,
ENGLAND
SN 1463-9076
EI 1463-9084
J9 PHYS CHEM CHEM PHYS
JI Phys. Chem. Chem. Phys.
PD OCT 14
PY 2016
VL 18
IS 38
BP 26423
EP 26433
DI 10.1039/c6cp03970g
PG 11
WC Chemistry, Physical; Physics, Atomic, Molecular & Chemical
SC Chemistry; Physics
GA DY5WL
UT WOS:000385175000010
PM 27711478
ER
PT J
AU Xie, H
Zou, JH
Kong, XT
Zhang, WQ
Ahmed, M
Jiang, L
AF Xie, Hua
Zou, Jinghan
Kong, Xiangtao
Zhang, Weiqing
Ahmed, Musahid
Jiang, Ling
TI Probing the microhydration of metal carbonyls: a photoelectron
velocity-map imaging spectroscopic and theoretical study of
Ni(CO)(3)(H2O)n(-)
SO PHYSICAL CHEMISTRY CHEMICAL PHYSICS
LA English
DT Article
ID DENSITY-FUNCTIONAL CALCULATIONS; MATRIX INFRARED-SPECTRA; VIBRATIONAL
SPECTROSCOPY; CLUSTERS; TRANSITION; CO; ANIONS; ATOMS; CHEMISORPTION;
ADSORPTION
AB A series of microhydrated nickel carbonyls, Ni(CO)(3)(H2O)n(-) (n = 0-4), are prepared via a laser vaporization supersonic cluster source in the gas phase and identified by mass-selected photoelectron velocity-map imaging spectroscopy and quantum chemical calculations. Vertical detachment energies for the n = 1-4 anions are measured from the photoelectron spectra to be 1.429 +/- 0.103, 1.698 +/- 0.090, 1.887 +/- 0.080, and 2.023 +/- 0.074 eV, respectively. The C-O stretching vibrational frequencies in the corresponding neutral clusters are determined to be 1968, 1950, 1945, and 1940 cm(-1) for n = 1-4, respectively, which are characteristic of terminal CO. It is determined that the hydrogen atom of the first water molecule is bound to the nickel center. Addition of a second water molecule prefers solvation at the carbonyl terminal. Spectroscopy combined with theory suggests that the solvation of nickel tricarbonyl is dominated by a water-ring network. The present findings would have important implications for the fundamental understanding of the multifaceted mechanisms of the multibody interaction of water and carbon monoxide with transition metals.
C1 [Xie, Hua; Zou, Jinghan; Kong, Xiangtao; Zhang, Weiqing; Jiang, Ling] Chinese Acad Sci, Dalian Inst Chem Phys, Collaborat Innovat Ctr Chem Energy & Mat iChEM, State Key Lab Mol React Dynam, 457 Zhongshan Rd, Dalian 116023, Liaoning, Peoples R China.
[Ahmed, Musahid] Lawrence Berkeley Natl Lab, Div Chem Sci, Berkeley, CA 94720 USA.
RP Jiang, L (reprint author), Chinese Acad Sci, Dalian Inst Chem Phys, Collaborat Innovat Ctr Chem Energy & Mat iChEM, State Key Lab Mol React Dynam, 457 Zhongshan Rd, Dalian 116023, Liaoning, Peoples R China.
EM ljiang@dicp.ac.cn
FU National Natural Science Foundation of China [21273233, 21327901,
21503222]; Key Research Programme of the Chinese Academy of Science
[KGZD-EW-T05]; Chinese Academy of Sciences; Office of Science, Office of
Basic Energy Sciences, of the U.S. Department of Energy under Chemical
Sciences Division [DE-AC02-05CH11231]
FX This work was supported by the National Natural Science Foundation of
China (Grant No. 21273233, 21327901, and 21503222) and the Key Research
Programme of the Chinese Academy of Science (Grant No. KGZD-EW-T05). L.
J. acknowledges the Hundred Talents Program of Chinese Academy of
Sciences. M. A. is supported by the Director, Office of Science, Office
of Basic Energy Sciences, of the U.S. Department of Energy under
Contract No. DE-AC02-05CH11231, through the Chemical Sciences Division.
NR 36
TC 0
Z9 0
U1 11
U2 11
PU ROYAL SOC CHEMISTRY
PI CAMBRIDGE
PA THOMAS GRAHAM HOUSE, SCIENCE PARK, MILTON RD, CAMBRIDGE CB4 0WF, CAMBS,
ENGLAND
SN 1463-9076
EI 1463-9084
J9 PHYS CHEM CHEM PHYS
JI Phys. Chem. Chem. Phys.
PD OCT 14
PY 2016
VL 18
IS 38
BP 26719
EP 26724
DI 10.1039/c6cp05035b
PG 6
WC Chemistry, Physical; Physics, Atomic, Molecular & Chemical
SC Chemistry; Physics
GA DY5WL
UT WOS:000385175000040
PM 27711570
ER
PT J
AU Fagiani, MR
Knorke, H
Esser, TK
Heine, N
Wolke, CT
Gewinner, S
Schollkopf, W
Gaigeot, MP
Spezia, R
Johnson, MA
Asmis, KR
AF Fagiani, Matias R.
Knorke, Harald
Esser, Tim K.
Heine, Nadja
Wolke, Conrad T.
Gewinner, Sandy
Schoellkopf, Wieland
Gaigeot, Marie-Pierre
Spezia, Riccardo
Johnson, Mark A.
Asmis, Knut R.
TI Gas phase vibrational spectroscopy of the protonated water pentamer: the
role of isomers and nuclear quantum effects
SO PHYSICAL CHEMISTRY CHEMICAL PHYSICS
LA English
DT Article
ID GAUSSIAN-BASIS SETS; INFRARED-SPECTROSCOPY; MOLECULAR CALCULATIONS;
SPECTRAL SIGNATURES; IR SPECTROSCOPY; WAVE-FUNCTIONS; EXCESS PROTON;
ION-TRAP; CLUSTERS; DYNAMICS
AB We use cryogenic ion trap vibrational spectroscopy to study the structure of the protonated water pentamer, H+(H2O)(5), and its fully deuterated isotopologue, D+(D2O)(5), over nearly the complete infrared spectral range (220-4000 cm(-1)) in combination with harmonic and anharmonic electronic structure calculations as well as RRKM modelling. Isomer-selective IR-IR double-resonance measurements on the H+(H2O)(5) isotopologue establish that the spectrum is due to a single constitutional isomer, thus discounting the recent analysis of the band pattern in the context of two isomers based on AIMD simulations < W. Kulig and N. Agmon, Phys. Chem. Chem. Phys., 2014, 16, 4933-4941 >. The evolution of the persistent bands in the D+(D2O)(5) cluster allows the assignment of the fundamentals in the spectra of both isotopologues, and the simpler pattern displayed by the heavier isotopologue is consistent with the calculated spectrum for the branched, Eigen-based structure originally proposed < J.-C. Jiang, et al., J. Am. Chem. Soc., 2000, 122, 1398-1410 >. This pattern persists in the vibrational spectra of H+(H2O)(5) in the temperature range from 13 K up to 250 K. The present study also underscores the importance of considering nuclear quantum effects in predicting the kinetic stability of these isomers at low temperatures.
C1 [Fagiani, Matias R.; Knorke, Harald; Esser, Tim K.; Asmis, Knut R.] Univ Leipzig, Wilhelm Ostwald Inst Phys & Theoret Chem, Linnestr 2, D-04103 Leipzig, Germany.
[Fagiani, Matias R.; Heine, Nadja; Gewinner, Sandy; Schoellkopf, Wieland] Fritz Haber Inst Max Planck Gesell, Faradayweg 4-6, D-14195 Berlin, Germany.
[Wolke, Conrad T.; Johnson, Mark A.] Yale Univ, Dept Chem, New Haven, CT 06520 USA.
[Gaigeot, Marie-Pierre; Spezia, Riccardo] Univ Evry Val Essonne, UMR 8587, LAMBE, Blvd F Mitterrand, F-91025 Evry, France.
[Gaigeot, Marie-Pierre; Spezia, Riccardo] CNRS, Lab Anal & Modelisat Biol & Environm, UMR 8587, F-91025 Evry, France.
[Heine, Nadja] Lawrence Berkeley Natl Lab, Div Chem Sci, Berkeley, CA 94720 USA.
RP Asmis, KR (reprint author), Univ Leipzig, Wilhelm Ostwald Inst Phys & Theoret Chem, Linnestr 2, D-04103 Leipzig, Germany.
EM knut.asmis@uni-leipzig.de
RI Asmis, Knut/N-5408-2014;
OI Asmis, Knut/0000-0001-6297-5856; spezia, riccardo/0000-0001-5160-489X
FU Collaborative Research Center of the German Research Foundation DFG
[1109]; U.S. Department of Energy [DE-FG02-06ER15800]
FX This research is supported by the Collaborative Research Center 1109 of
the German Research Foundation DFG. MAJ thanks the U.S. Department of
Energy under grant DE-FG02-06ER15800.
NR 50
TC 5
Z9 5
U1 19
U2 19
PU ROYAL SOC CHEMISTRY
PI CAMBRIDGE
PA THOMAS GRAHAM HOUSE, SCIENCE PARK, MILTON RD, CAMBRIDGE CB4 0WF, CAMBS,
ENGLAND
SN 1463-9076
EI 1463-9084
J9 PHYS CHEM CHEM PHYS
JI Phys. Chem. Chem. Phys.
PD OCT 14
PY 2016
VL 18
IS 38
BP 26743
EP 26754
DI 10.1039/c6cp05217g
PG 12
WC Chemistry, Physical; Physics, Atomic, Molecular & Chemical
SC Chemistry; Physics
GA DY5WL
UT WOS:000385175000043
PM 27722600
ER
PT J
AU Lobaccaro, P
Singh, MR
Clark, EL
Kwon, Y
Bell, AT
Ager, JW
AF Lobaccaro, Peter
Singh, Meenesh R.
Clark, Ezra Lee
Kwon, Youngkook
Bell, Alexis T.
Ager, Joel W.
TI Effects of temperature and gas-liquid mass transfer on the operation of
small electrochemical cells for the quantitative evaluation of CO2
reduction electrocatalysts
SO PHYSICAL CHEMISTRY CHEMICAL PHYSICS
LA English
DT Article
ID BUBBLE-COLUMN REACTORS; CARBON-DIOXIDE REDUCTION; AQUEOUS
HYDROGENCARBONATE SOLUTION; COPPER ELECTRODE; TRANSFER COEFFICIENT;
SALT-SOLUTIONS; DISSOCIATION-CONSTANTS; IONIZATION-CONSTANT;
HYDROGEN-PRODUCTION; METAL-ELECTRODES
AB In the last few years, there has been increased interest in electrochemical CO2 reduction (CO2R). Many experimental studies employ a membrane separated, electrochemical cell with a mini H-cell geometry to characterize CO2R catalysts in aqueous solution. This type of electrochemical cell is a mini-chemical reactor and it is important to monitor the reaction conditions within the reactor to ensure that they are constant throughout the study. We show that operating cells with high catalyst surface area to electrolyte volume ratios (S/V) at high current densities can have subtle consequences due to the complexity of the physical phenomena taking place on electrode surfaces during CO2R, particularly as they relate to the cell temperature and bulk electrolyte CO2 concentration. Both effects were evaluated quantitatively in high S/V cells using Cu electrodes and a bicarbonate buffer electrolyte. Electrolyte temperature is a function of the current/total voltage passed through the cell and the cell geometry. Even at a very high current density, 20 mA cm(-2), the temperature increase was less than 4 degrees C and a decrease of <10% in the dissolved CO2 concentration is predicted. In contrast, limits on the CO2 gas-liquid mass transfer into the cells produce much larger effects. By using the pH in the cell to measure the CO2 concentration, significant undersaturation of CO2 is observed in the bulk electrolyte, even at more modest current densities of 10 mA cm(-2). Undersaturation of CO2 produces large changes in the faradaic efficiency observed on Cu electrodes, with H-2 production becoming increasingly favored. We show that the size of the CO2 bubbles being introduced into the cell is critical for maintaining the equilibrium CO2 concentration in the electrolyte, and we have designed a high S/V cell that is able to maintain the near-equilibrium CO2 concentration at current densities up to 15 mA cm(-2).
C1 [Lobaccaro, Peter; Singh, Meenesh R.; Clark, Ezra Lee; Kwon, Youngkook; Bell, Alexis T.; Ager, Joel W.] Lawrence Berkeley Natl Lab, Joint Ctr Artificial Photosynth, Berkeley, CA 94720 USA.
[Lobaccaro, Peter; Singh, Meenesh R.; Clark, Ezra Lee; Kwon, Youngkook; Bell, Alexis T.] Lawrence Berkeley Natl Lab, Div Chem Sci, Berkeley, CA 94720 USA.
[Lobaccaro, Peter; Singh, Meenesh R.; Clark, Ezra Lee; Bell, Alexis T.] Univ Calif Berkeley, Dept Chem & Biomol Engn, Berkeley, CA 94720 USA.
[Ager, Joel W.] Lawrence Berkeley Natl Lab, Div Mat Sci, Berkeley, CA 94720 USA.
[Ager, Joel W.] Univ Calif Berkeley, Dept Mat Sci & Engn, Berkeley, CA 94720 USA.
RP Bell, AT; Ager, JW (reprint author), Lawrence Berkeley Natl Lab, Joint Ctr Artificial Photosynth, Berkeley, CA 94720 USA.; Bell, AT (reprint author), Lawrence Berkeley Natl Lab, Div Chem Sci, Berkeley, CA 94720 USA.; Bell, AT (reprint author), Univ Calif Berkeley, Dept Chem & Biomol Engn, Berkeley, CA 94720 USA.; Ager, JW (reprint author), Lawrence Berkeley Natl Lab, Div Mat Sci, Berkeley, CA 94720 USA.; Ager, JW (reprint author), Univ Calif Berkeley, Dept Mat Sci & Engn, Berkeley, CA 94720 USA.
EM alexbell@berkeley.edu; jwager@lbl.gov
OI Singh, Meenesh/0000-0002-3638-8866
FU California Energy Commission [500-11-023]; Office of Science of the U.S.
Department of Energy [DE-SC0004993]; National Science Foundation
Graduate Fellowship
FX Initial fabrication and cell design testing were supported by the
California Energy Commission under agreement 500-11-023. Detailed CO2R
testing and modelling of the electrochemical cell were performed within
the Joint Center for Artificial Photosynthesis, a DOE Energy Innovation
Hub, supported through the Office of Science of the U.S. Department of
Energy under Award Number DE-SC0004993. EC acknowledges support from the
National Science Foundation Graduate Fellowship. We thank Eric Granlund,
the manager of the Berkeley College of Chemistry Machine Shop, for his
expertise in machining and cell fabrication and Yanwei Lum for helpful
discussions. We thank Adams and Chittenden Scientific Glass for their
assistance in designing the frit unit.
NR 82
TC 0
Z9 0
U1 19
U2 19
PU ROYAL SOC CHEMISTRY
PI CAMBRIDGE
PA THOMAS GRAHAM HOUSE, SCIENCE PARK, MILTON RD, CAMBRIDGE CB4 0WF, CAMBS,
ENGLAND
SN 1463-9076
EI 1463-9084
J9 PHYS CHEM CHEM PHYS
JI Phys. Chem. Chem. Phys.
PD OCT 14
PY 2016
VL 18
IS 38
BP 26777
EP 26785
DI 10.1039/c6cp05287h
PG 9
WC Chemistry, Physical; Physics, Atomic, Molecular & Chemical
SC Chemistry; Physics
GA DY5WL
UT WOS:000385175000047
PM 27722320
ER
PT J
AU Weck, PF
Kim, E
AF Weck, Philippe F.
Kim, Eunja
TI Assessing Hubbard-corrected AM05+U and PBEsol plus U density functionals
for strongly correlated oxides CeO2 and Ce2O3
SO PHYSICAL CHEMISTRY CHEMICAL PHYSICS
LA English
DT Article
ID GENERALIZED GRADIENT APPROXIMATION; BRILLOUIN-ZONE INTEGRATIONS;
MEAN-FIELD THEORY; CERIA; NANOPARTICLES; NANOCRYSTALS; TEMPERATURE;
STABILITY; PRESSURE; SURFACES
AB The structure-property relationships of bulk CeO2 and Ce2O3 have been investigated using AM05 and PBEsol exchange-correlation functionals within the frameworks of Hubbard-corrected density functional theory (DFT+U) and density functional perturbation theory (DFPT+U). Compared with conventional PBE+U, RPBE+U, PW91+U and LDA+U functionals, AM05+U and PBEsol+U describe experimental crystalline parameters and properties of CeO2 and Ce2O3 with superior accuracy, especially when +U is chosen close to its value derived by the linear-response approach. The present findings call for a reexamination of some of the problematic oxide materials featuring strong f- and d-electron correlation using AM05+U and PBEsol+U.
C1 [Weck, Philippe F.] Sandia Natl Labs, POB 5800, Albuquerque, NM 87185 USA.
[Kim, Eunja] Univ Nevada, Dept Phys & Astron, Las Vegas, NV 89154 USA.
RP Weck, PF (reprint author), Sandia Natl Labs, POB 5800, Albuquerque, NM 87185 USA.
EM pfweck@sandia.gov
FU U.S. Department of Energy's National Nuclear Security Administration
[DE-AC04-94AL85000]; Sandia National Laboratories
FX Sandia National Laboratories is a multi-program laboratory managed and
operated by Sandia Corporation, a wholly owned subsidiary of Lockheed
Martin Corporation, for the U.S. Department of Energy's National Nuclear
Security Administration under contract DE-AC04-94AL85000. This work was
supported Laboratory Directed Research and Development (LDRD) funding
from Sandia National Laboratories.
NR 74
TC 0
Z9 0
U1 9
U2 9
PU ROYAL SOC CHEMISTRY
PI CAMBRIDGE
PA THOMAS GRAHAM HOUSE, SCIENCE PARK, MILTON RD, CAMBRIDGE CB4 0WF, CAMBS,
ENGLAND
SN 1463-9076
EI 1463-9084
J9 PHYS CHEM CHEM PHYS
JI Phys. Chem. Chem. Phys.
PD OCT 14
PY 2016
VL 18
IS 38
BP 26816
EP 26826
DI 10.1039/c6cp05479j
PG 11
WC Chemistry, Physical; Physics, Atomic, Molecular & Chemical
SC Chemistry; Physics
GA DY5WL
UT WOS:000385175000051
PM 27711607
ER
PT J
AU Christov, IC
Viswanathan, HS
AF Christov, Ivan C.
Viswanathan, Hari S.
TI Introduction: energy and the subsurface
SO PHILOSOPHICAL TRANSACTIONS OF THE ROYAL SOCIETY A-MATHEMATICAL PHYSICAL
AND ENGINEERING SCIENCES
LA English
DT Article
DE energy; subsurface; mechanics; hydraulic fracturing; carbon
sequestration; porous media
AB This theme issue covers topics at the forefront of scientific research on energy and the subsurface, ranging from carbon dioxide (CO2) sequestration to the recovery of unconventional shale oil and gas resources through hydraulic fracturing. As such, the goal of this theme issue is to have an impact on the scientific community, broadly, by providing a self-contained collection of articles contributing to and reviewing the state-of-the-art of the field. This collection of articles could be used, for example, to set the next generation of research directions, while also being useful as a self-study guide for those interested in entering the field. Review articles are included on the topics of hydraulic fracturing as a multiscale problem, numerical modelling of hydraulic fracture propagation, the role of computational sciences in the upstream oil and gas industry and chemohydrodynamic patterns in porous media. Complementing the reviews is a set of original research papers covering growth models for branched hydraulic crack systems, fluid-driven crack propagation in elastic matrices, elastic and inelastic deformation of fluid-saturated rock, reaction front propagation in fracture matrices, the effects of rock mineralogy and pore structure on stress-dependent permeability of shales, topographic viscous fingering and plume dynamics in porous media convection.
This article is part of the themed issue 'Energy and the subsurface'.
C1 [Christov, Ivan C.] Purdue Univ, Sch Mech Engn, W Lafayette, IN 47907 USA.
[Viswanathan, Hari S.] Los Alamos Natl Lab, Earth & Environm Sci, Los Alamos, NM 87545 USA.
RP Christov, IC (reprint author), Purdue Univ, Sch Mech Engn, W Lafayette, IN 47907 USA.
EM christov@purdue.edu
RI Christov, Ivan/B-9418-2008
OI Christov, Ivan/0000-0001-8531-0531
FU Los Alamos National Laboratory's Laboratory Directed Research and
Development (LDRD) programme through the Center for Nonlinear Studies;
Los Alamos National Laboratory's Laboratory Directed Research and
Development (LDRD) programme [20140002DR]; National Nuclear Security
Administration of the US Department of Energy [DE-AC52-06NA25396]
FX We gratefully acknowledge support from Los Alamos National Laboratory's
Laboratory Directed Research and Development (LDRD) programme through
the Center for Nonlinear Studies and grant no. 20140002DR. Los Alamos
National Laboratory is operated by Los Alamos National Security LLC for
the National Nuclear Security Administration of the US Department of
Energy under contract no. DE-AC52-06NA25396.
NR 13
TC 0
Z9 0
U1 4
U2 4
PU ROYAL SOC
PI LONDON
PA 6-9 CARLTON HOUSE TERRACE, LONDON SW1Y 5AG, ENGLAND
SN 1364-503X
EI 1471-2962
J9 PHILOS T R SOC A
JI Philos. Trans. R. Soc. A-Math. Phys. Eng. Sci.
PD OCT 13
PY 2016
VL 374
IS 2078
AR 20150430
DI 10.1098/rsta.2015.0430
PG 6
WC Multidisciplinary Sciences
SC Science & Technology - Other Topics
GA EG6EW
UT WOS:000391138300012
ER
PT J
AU Ecke, RE
Backhaus, S
AF Ecke, Robert E.
Backhaus, Scott
TI Plume dynamics in Hele-Shaw porous media convection
SO PHILOSOPHICAL TRANSACTIONS OF THE ROYAL SOCIETY A-MATHEMATICAL PHYSICAL
AND ENGINEERING SCIENCES
LA English
DT Article
DE porous media; convection; plume dynamics
ID CARBON-DIOXIDE; ONSET; STABILITY; STORAGE
AB Mass transport in multi-species porous media is through molecular diffusion and plume dynamics. Predicting the rate of mass transport has application in determining the efficiency of the storage and sequestration of carbon dioxide. We study a water and propylene-glycol system enclosed in a Hele-Shaw cell with variable permeability that represents a laboratory analogue of the general properties of porous media convection. The interface between the fluids, tracked using an optical shadowgraph technique, is used to determine the mass transport rate, the spatial separation of solutal plumes, and the velocity and width characteristics of those plumes. One finds that the plume dynamics are closely related to the mass transport rate.
This article is part of the themed issue 'Energy and the subsurface'.
C1 [Ecke, Robert E.] MPA CMMS, Los Alamos, NM 87545 USA.
[Ecke, Robert E.] CNLS, Los Alamos, NM 87545 USA.
[Backhaus, Scott] Los Alamos Natl Lab, A-1, Los Alamos, NM 87545 USA.
RP Ecke, RE (reprint author), MPA CMMS, Los Alamos, NM 87545 USA.; Ecke, RE (reprint author), CNLS, Los Alamos, NM 87545 USA.
EM ecke@lanl.gov
OI Backhaus, Scott/0000-0002-0344-6791; Ecke, Robert/0000-0001-7772-5876
FU National Nuclear Security Administration of the US Department of Energy
at Los Alamos National Laboratory [DE-AC52-06NA25396]
FX This work was carried out under the auspices of the National Nuclear
Security Administration of the US Department of Energy at Los Alamos
National Laboratory under contract no. DE-AC52-06NA25396.
NR 17
TC 2
Z9 2
U1 0
U2 0
PU ROYAL SOC
PI LONDON
PA 6-9 CARLTON HOUSE TERRACE, LONDON SW1Y 5AG, ENGLAND
SN 1364-503X
EI 1471-2962
J9 PHILOS T R SOC A
JI Philos. Trans. R. Soc. A-Math. Phys. Eng. Sci.
PD OCT 13
PY 2016
VL 374
IS 2078
AR 20150420
DI 10.1098/rsta.2015.0420
PG 11
WC Multidisciplinary Sciences
SC Science & Technology - Other Topics
GA EG6EW
UT WOS:000391138300003
ER
PT J
AU Hyman, JD
Jimenez-Martinez, J
Viswanathan, HS
Carey, JW
Porter, ML
Rougier, E
Karra, S
Kang, Q
Frash, L
Chen, L
Lei, Z
O'Malley, D
Makedonska, N
AF Hyman, J. D.
Jimenez-Martinez, J.
Viswanathan, H. S.
Carey, J. W.
Porter, M. L.
Rougier, E.
Karra, S.
Kang, Q.
Frash, L.
Chen, L.
Lei, Z.
O'Malley, D.
Makedonska, N.
TI Understanding hydraulic fracturing: a multi-scale problem
SO PHILOSOPHICAL TRANSACTIONS OF THE ROYAL SOCIETY A-MATHEMATICAL PHYSICAL
AND ENGINEERING SCIENCES
LA English
DT Review
DE hydraulic fracturing; shale gas; subsurface flow and transport; discrete
fracture network; lattice Boltzmann; microfluidics
ID LATTICE BOLTZMANN METHOD; DISCRETE ELEMENT METHOD; HYBRID MORTAR METHOD;
SHALE-GAS; TRANSPORT-PROPERTIES; CARBON-DIOXIDE; SOLVING FLOW; NETWORKS;
PERMEABILITY; SUBSURFACE
AB Despite the impact that hydraulic fracturing has had on the energy sector, the physical mechanisms that control its efficiency and environmental impacts remain poorly understood in part because the length scales involved range from nanometres to kilometres. We characterize flow and transport in shale formations across and between these scales using integrated computational, theoretical and experimental efforts/methods. At the field scale, we use discrete fracture network modelling to simulate production of a hydraulically fractured well from a fracture network that is based on the site characterization of a shale gas reservoir. At the core scale, we use triaxial fracture experiments and a finite-discrete element model to study dynamic fracture/crack propagation in low permeability shale. We use lattice Boltzmann pore-scale simulations and microfluidic experiments in both synthetic and shale rock micromodels to study pore-scale flow and transport phenomena, including multi-phase flow and fluids mixing. A mechanistic description and integration of these multiple scales is required for accurate predictions of production and the eventual optimization of hydrocarbon extraction from unconventional reservoirs. Finally, we discuss the potential of CO2 as an alternative working fluid, both in fracturing and re-stimulating activities, beyond its environmental advantages.
This article is part of the themed issue 'Energy and the subsurface'.
C1 [Hyman, J. D.; Jimenez-Martinez, J.; Viswanathan, H. S.; Carey, J. W.; Porter, M. L.; Rougier, E.; Karra, S.; Kang, Q.; Frash, L.; Chen, L.; Lei, Z.; O'Malley, D.; Makedonska, N.] Los Alamos Natl Lab, Earth & Environm Sci, Los Alamos, NM 87544 USA.
RP Viswanathan, HS (reprint author), Los Alamos Natl Lab, Earth & Environm Sci, Los Alamos, NM 87544 USA.
EM viswana@lanl.gov
OI Frash, Luke/0000-0002-5424-4698; Lei, Zhou/0000-0002-4965-5556;
Jimenez-Martinez, Joaquin/0000-0002-2063-6490; Makedonska,
Nataliia/0000-0002-4183-5755; Hyman, Jeffrey /0000-0002-4224-2847;
Karra, Satish/0000-0001-7847-6293; O'Malley, Daniel/0000-0003-0432-3088
FU LANL's DR research programme [20140002DR]; LANL Director's Post Doctoral
Fellowship
FX We are grateful for support from LANL's DR research programme, grant no.
20140002DR. Q.K. thanks DOE-NETL Unconventional Oil & Gas. J.D.H., L.C.,
L.F. and D.O. acknowledge the support of the LANL Director's Post
Doctoral Fellowship.
NR 64
TC 1
Z9 1
U1 14
U2 14
PU ROYAL SOC
PI LONDON
PA 6-9 CARLTON HOUSE TERRACE, LONDON SW1Y 5AG, ENGLAND
SN 1364-503X
EI 1471-2962
J9 PHILOS T R SOC A
JI Philos. Trans. R. Soc. A-Math. Phys. Eng. Sci.
PD OCT 13
PY 2016
VL 374
IS 2078
AR 20150426
DI 10.1098/rsta.2015.0426
PG 16
WC Multidisciplinary Sciences
SC Science & Technology - Other Topics
GA EG6EW
UT WOS:000391138300008
ER
PT J
AU Hess, BM
Amidan, BG
Anderson, KK
Hutchison, JR
AF Hess, Becky M.
Amidan, Brett G.
Anderson, Kevin K.
Hutchison, Janine R.
TI Evaluating Composite Sampling Methods of Bacillus Spores at Low
Concentrations
SO PLOS ONE
LA English
DT Article
ID ANTHRACIS DELTA-STERNE; NONPOROUS SURFACES; RECOVERY; DECONTAMINATION;
COLLECTION; PROTOCOL
AB Restoring all facility operations after the 2001 Amerithrax attacks took years to complete, highlighting the need to reduce remediation time. Some of the most time intensive tasks were environmental sampling and sample analyses. Composite sampling allows disparate samples to be combined, with only a single analysis needed, making it a promising method to reduce response times. We developed a statistical experimental design to test three different composite sampling methods: 1) single medium single pass composite (SM-SPC): a single cellulose sponge samples multiple coupons with a single pass across each coupon; 2) single medium multi-pass composite: a single cellulose sponge samples multiple coupons with multiple passes across each coupon (SM-MPC); and 3) multi-medium post-sample composite (MM-MPC): a single cellulose sponge samples a single surface, and then multiple sponges are combined during sample extraction. Five spore concentrations of Bacillus atrophaeus Nakamura spores were tested; concentrations ranged from 5 to 100 CFU/coupon (0.00775 to 0.155 CFU/cm(2)). Study variables included four clean surface materials (stainless steel, vinyl tile, ceramic tile, and painted dry wallboard) and three grime coated/dirty materials (stainless steel, vinyl tile, and ceramic tile). Analysis of variance for the clean study showed two significant factors: composite method (p<0.0001) and coupon material (p = 0.0006). Recovery efficiency (RE) was higher overall using the MM-MPC method compared to the SM-SPC and SM-MPC methods. RE with the MM-MPC method for concentrations tested (10 to 100 CFU/coupon) was similar for ceramic tile, dry wall, and stainless steel for clean materials. RE was lowest for vinyl tile with both composite methods. Statistical tests for the dirty study showed RE was significantly higher for vinyl and stainless steel materials, but lower for ceramic tile. These results suggest post-sample compositing can be used to reduce sample analysis time when responding to a Bacillus anthracis contamination event of clean or dirty surfaces.
C1 [Hess, Becky M.; Amidan, Brett G.; Anderson, Kevin K.; Hutchison, Janine R.] Pacific Northwest Natl Lab, Natl Secur Directorate, Richland, WA 99352 USA.
RP Hutchison, JR (reprint author), Pacific Northwest Natl Lab, Natl Secur Directorate, Richland, WA 99352 USA.
EM Janine.Hutchison@pnnl.gov
FU Chemical and Biological Research; Development Branch of the Chemical and
Biological Division in the Science and Technology Directorate of the
Department of Homeland Security (DHS)
FX The Pacific Northwest National Laboratory (PNNL) work was funded by the
Chemical and Biological Research and Development Branch of the Chemical
and Biological Division in the Science and Technology Directorate of the
Department of Homeland Security (DHS). PR#: RSRD-14-XXXX,
https://www.dhs.gov/science-and-technology/st-cbd. The funders had no
role in study design, data collection and analysis, decision to publish,
or preparation of the manuscript.
NR 25
TC 0
Z9 0
U1 3
U2 3
PU PUBLIC LIBRARY SCIENCE
PI SAN FRANCISCO
PA 1160 BATTERY STREET, STE 100, SAN FRANCISCO, CA 94111 USA
SN 1932-6203
J9 PLOS ONE
JI PLoS One
PD OCT 13
PY 2016
VL 11
IS 10
AR e0164582
DI 10.1371/journal.pone.0164582
PG 22
WC Multidisciplinary Sciences
SC Science & Technology - Other Topics
GA DZ0CV
UT WOS:000385505800089
PM 27736999
ER
PT J
AU He, YM
Thorne, JE
Wu, CH
Ma, PY
Du, C
Dong, Q
Guo, JH
Wang, DW
AF He, Yumin
Thorne, James E.
Wu, Cheng Hao
Ma, Peiyan
Du, Chun
Dong, Qi
Guo, Jinghua
Wang, Dunwei
TI What Limits the Performance of Ta3N5 for Solar Water Splitting?
SO CHEM
LA English
DT Article
ID NANOTUBE PHOTOANODES; NANOROD ARRAYS; LAYER; PHOTOELECTRODES; CATALYST;
SURFACE; PHOTOCATALYST; POSITIONS; JUNCTIONS; STATES
AB Tantalum nitride (Ta3N5) is a promising photoelectrode for solar water splitting. Although near-theoretical-limit photocurrent has already been reported on Ta3N5, its low photovoltage and poor stability remain critical challenges. In this study, we used Ta3N5 nanotubes as a platform to understand the origins of these issues. Through a combination of photoelectrochemical and high-resolution electron microscope measurements, we found that the self-limiting surface oxidation of Ta3N5 resulted in a thin amorphous layer (ca. 3 nm), which proved to be effective in pinning the surface Fermi levels and thus fully suppressed the photoactivity of Ta3N5. X-ray core-level spectroscopy characterization not only confirmed the surface composition change resulting from the oxidation but also revealed a Fermi-level shift toward the positive direction by up to 0.5 V. The photoactivity degradation mechanism reported here is likely to find applications in other solar-to-chemical energy-conversion systems.
C1 [He, Yumin; Thorne, James E.; Ma, Peiyan; Du, Chun; Dong, Qi; Wang, Dunwei] Boston Coll, Dept Chem, Merkert Chem Ctr, 2609 Beacon St, Chestnut Hill, MA 02467 USA.
[Wu, Cheng Hao; Guo, Jinghua] Lawrence Berkeley Natl Lab, Adv Light Source, Berkeley, CA 94720 USA.
[Ma, Peiyan] Wuhan Univ Technol, Sch Chem Chem Engn & Life Sci, Wuhan 430070, Hubei, Peoples R China.
RP Wang, DW (reprint author), Boston Coll, Dept Chem, Merkert Chem Ctr, 2609 Beacon St, Chestnut Hill, MA 02467 USA.
EM dunwei.wang@bc.edu
OI Thorne, James/0000-0002-7711-428X
NR 48
TC 0
Z9 0
U1 9
U2 9
PU CELL PRESS
PI CAMBRIDGE
PA 600 TECHNOLOGY SQUARE, 5TH FLOOR, CAMBRIDGE, MA 02139 USA
SN 2451-9294
J9 CHEM
JI Chem
PD OCT 13
PY 2016
VL 1
IS 4
BP 640
EP 655
DI 10.1016/j.chempr.2016.09.006
PG 16
WC Chemistry, Multidisciplinary
SC Chemistry
GA EB0LJ
UT WOS:000387035000015
ER
PT J
AU East-Seletsky, A
O'Connell, MR
Knight, SC
Burstein, D
Cate, JHD
Tjian, R
Doudna, JA
AF East-Seletsky, Alexandra
O'Connell, Mitchell R.
Knight, Spencer C.
Burstein, David
Cate, Jamie H. D.
Tjian, Robert
Doudna, Jennifer A.
TI Two distinct RNase activities of CRISPR-C2c2 enable guide-RNA processing
and RNA detection
SO NATURE
LA English
DT Article
ID CAS SYSTEMS; DUAL-RNA; DNA; ENDORIBONUCLEASE; PROTEIN; CLEAVAGE;
IMMUNITY; DEFENSE; COMPLEX; ENDONUCLEASE
AB Bacterial adaptive immune systems use CRISPRs (clustered regularly interspaced short palindromic repeats) and CRISPR-associated (Cas) proteins for RNA-guided nucleic acid cleavage(1,2). Although most prokaryotic adaptive immune systems generally target DNA substrates(3-5), type III and VI CRISPR systems direct interference complexes against single-stranded RNA substrates(6-9). In type VI systems, the single-subunit C2c2 protein functions as an RNA-guided RNA endonuclease (RNase)(9,10). How this enzyme acquires mature CRISPR RNAs (crRNAs) that are essential for immune surveillance and how it carries out crRNA-mediated RNA cleavage remain unclear. Here we show that bacterial C2c2 possesses a unique RNase activity responsible for CRISPR RNA maturation that is distinct from its RNA-activated single-stranded RNA degradation activity. These dual RNase functions are chemically and mechanistically different from each other and from the crRNA-processing behaviour of the evolutionarily unrelated CRISPR enzyme Cpf1 (ref. 11). The two RNase activities of C2c2 enable multiplexed processing and loading of guide RNAs that in turn allow sensitive detection of cellular transcripts.
C1 [East-Seletsky, Alexandra; O'Connell, Mitchell R.; Cate, Jamie H. D.; Tjian, Robert; Doudna, Jennifer A.] Univ Calif Berkeley, Dept Mol & Cell Biol, Berkeley, CA 94720 USA.
[Knight, Spencer C.; Cate, Jamie H. D.; Doudna, Jennifer A.] Univ Calif Berkeley, Dept Chem, Berkeley, CA 94720 USA.
[Burstein, David] Univ Calif Berkeley, Dept Earth & Planetary Sci, Berkeley, CA 94720 USA.
[Cate, Jamie H. D.; Doudna, Jennifer A.] Lawrence Berkeley Natl Lab, MBIB Div, Berkeley, CA 94720 USA.
[Tjian, Robert] Howard Hughes Med Inst, Janelia Res Campus, Ashburn, VA 20147 USA.
[Tjian, Robert; Doudna, Jennifer A.] Univ Calif Berkeley, Howard Hughes Med Inst, Berkeley, CA 94720 USA.
[Tjian, Robert] Univ Calif Berkeley, Li Ka Shing Biomed & Hlth Sci Ctr, Berkeley, CA 94720 USA.
[Doudna, Jennifer A.] Univ Calif Berkeley, Innovat Genom Initiat, Berkeley, CA 94720 USA.
RP Doudna, JA (reprint author), Univ Calif Berkeley, Dept Mol & Cell Biol, Berkeley, CA 94720 USA.; Doudna, JA (reprint author), Univ Calif Berkeley, Dept Chem, Berkeley, CA 94720 USA.; Doudna, JA (reprint author), Lawrence Berkeley Natl Lab, MBIB Div, Berkeley, CA 94720 USA.; Doudna, JA (reprint author), Univ Calif Berkeley, Howard Hughes Med Inst, Berkeley, CA 94720 USA.; Doudna, JA (reprint author), Univ Calif Berkeley, Innovat Genom Initiat, Berkeley, CA 94720 USA.
EM doudna@berkeley.edu
FU National Science Foundation Graduate Research Fellowship Program; C. J.
Martin Overseas Early Career Fellowship from the National Health and
Medical Research Council of Australia; Frontiers Science award from the
Paul Allen Institute; National Science Foundation [MCB-1244557];
California Institute for Regenerative Medicine (CIRM) [RB4-06016];
National Institutes of Health [P50-GM102706]
FX We thank the QB3 MacroLab for assistance with cloning of C2c2
constructs; N. Ma and K. Zhou for technical assistance; S. N. Floor, S.
C. Strutt, A. V. Wright and M. L. Hochstrasser for critical reading of
the manuscript; and members of the Doudna, Cate and Tjian laboratories
for discussions. S. C. K. acknowledges support from the National Science
Foundation Graduate Research Fellowship Program; M.R.O. is a recipient
of a C. J. Martin Overseas Early Career Fellowship from the National
Health and Medical Research Council of Australia. This work was
supported in part by a Frontiers Science award from the Paul Allen
Institute to J.A.D., the National Science Foundation (MCB-1244557 to
J.A.D.), the California Institute for Regenerative Medicine (CIRM,
RB4-06016 to R.T.), and the National Institutes of Health (P50-GM102706
to J.H.D.C). R.T. and J.A.D. are Investigators of the Howard Hughes
Medical Institute. J.A.D. is a co-founder of Caribou Biosciences, Editas
Medicine and Intellia Therapeutics and a scientific advisor to Caribou,
Intellia, eFFECTOR Therapeutics, and Driver. A.E.S., M.R.O., S.C.K.,
J.H.D.C. and J.A.D. have filed a patent application related to this
work.
NR 34
TC 13
Z9 13
U1 28
U2 28
PU NATURE PUBLISHING GROUP
PI LONDON
PA MACMILLAN BUILDING, 4 CRINAN ST, LONDON N1 9XW, ENGLAND
SN 0028-0836
EI 1476-4687
J9 NATURE
JI Nature
PD OCT 13
PY 2016
VL 538
IS 7624
BP 270
EP +
DI 10.1038/nature19802
PG 17
WC Multidisciplinary Sciences
SC Science & Technology - Other Topics
GA EA5OS
UT WOS:000386671000050
PM 27669025
ER
PT J
AU Dehollain, JP
Muhonen, JT
Blume-Kohout, R
Rudinger, KM
Gamble, JK
Nielsen, E
Laucht, A
Simmons, S
Kalra, R
Dzurak, AS
Morello, A
AF Dehollain, Juan P.
Muhonen, Juha T.
Blume-Kohout, Robin
Rudinger, Kenneth M.
Gamble, John King
Nielsen, Erik
Laucht, Arne
Simmons, Stephanie
Kalra, Rachpon
Dzurak, Andrew S.
Morello, Andrea
TI Optimization of a solid-state electron spin qubit using gate set
tomography
SO NEW JOURNAL OF PHYSICS
LA English
DT Article
DE quantum computing; silicon; tomography
ID QUANTUM ERROR-CORRECTION; SILICON; FIDELITY; READOUT
AB State of the art qubit systems are reaching the gate fidelities required for scalable quantum computation architectures. Further improvements in the fidelity of quantum gates demands characterization and benchmarking protocols that are efficient, reliable and extremely accurate. Ideally, a benchmarking protocol should also provide information on how to rectify residual errors. Gate set tomography (GST) is one such protocol designed to give detailed characterization of as-built qubits. Weimplemented GST on a high-fidelity electron-spin qubit confined by a single P-31 atom in Si-28. The results reveal systematic errors that a randomized benchmarking analysis could measure but not identify, whereas GST indicated the need for improved calibration of the length of the control pulses. After introducing this modification, we measured a new benchmark average gate fidelity of 99.942(8)%, an improvement on the previous value of 99.90(2)%. Furthermore, GST revealed high levels of non-Markovian noise in the system, which will need to be understood and addressed when the qubit is used within a fault-tolerant quantum computation scheme.
C1 [Dehollain, Juan P.; Muhonen, Juha T.; Laucht, Arne; Simmons, Stephanie; Kalra, Rachpon; Dzurak, Andrew S.; Morello, Andrea] UNSW Australia, Sch Elect Engn & Telecommun, Ctr Quantum Computat & Commun Technol, Sydney, NSW 2052, Australia.
[Blume-Kohout, Robin; Rudinger, Kenneth M.; Gamble, John King; Nielsen, Erik] Sandia Natl Labs, POB 5800, Albuquerque, NM 87185 USA.
[Blume-Kohout, Robin; Rudinger, Kenneth M.; Gamble, John King] Sandia Natl Labs, Ctr Res Comp, POB 5800, Albuquerque, NM 87185 USA.
[Dehollain, Juan P.] Delft Univ Technol, QuTech, NL-2628 CJ Delft, Netherlands.
[Dehollain, Juan P.] Delft Univ Technol, Kavli Inst Nanosci, NL-2628 CJ Delft, Netherlands.
[Muhonen, Juha T.] FOM Inst AMOLF, Ctr Nanophoton, NL-1098 XG Amsterdam, Netherlands.
[Simmons, Stephanie] Simon Fraser Univ, Dept Phys, Burnaby, BC V5A 1S6, Canada.
RP Dehollain, JP (reprint author), UNSW Australia, Sch Elect Engn & Telecommun, Ctr Quantum Computat & Commun Technol, Sydney, NSW 2052, Australia.; Dehollain, JP (reprint author), Delft Univ Technol, QuTech, NL-2628 CJ Delft, Netherlands.; Dehollain, JP (reprint author), Delft Univ Technol, Kavli Inst Nanosci, NL-2628 CJ Delft, Netherlands.
EM j.p.dehollainlorenzana@tudelft.nl; enielse@sandia.gov;
a.morello@unsw.edu.au
RI Morello, Andrea/B-6475-2008; Muhonen, Juha/E-7152-2011;
OI Morello, Andrea/0000-0001-7445-699X; Muhonen, Juha/0000-0001-6520-6999;
Dehollain, Juan Pablo/0000-0002-0425-4345
FU Australian Research Council Centre of Excellence for Quantum Computation
and Communication Technology [CE110001027]; US Army Research Office
[W911NF-13-1-0024]; Australian National Fabrication Facility; US
Department of Energys National Nuclear Security Administration
[DE-AC04-94AL85000]; Sandia National Laboratories Truman Fellowship
Program - Laboratory Directed Research and Development (LDRD) program
FX We thank F Hudson for assistance in device fabrication and design, K
Itoh for supplying the 28Si epilayer, and J McCallum and D
Jamieson for the 31P donor implantation. This research was
funded by the Australian Research Council Centre of Excellence for
Quantum Computation and Communication Technology (project no.
CE110001027) and the US Army Research Office (W911NF-13-1-0024). The
authors acknowledge support from the Australian National Fabrication
Facility. Sandia National Laboratories is a multi-program laboratory
managed and operated by Sandia Corporation, a wholly owned subsidiary of
Lockheed Martin Corporation, for the US Department of Energys National
Nuclear Security Administration under contract DE-AC04-94AL85000. JKG
gratefully acknowledges support from the Sandia National Laboratories
Truman Fellowship Program, which is funded by the Laboratory Directed
Research and Development (LDRD) program.
NR 42
TC 0
Z9 0
U1 6
U2 6
PU IOP PUBLISHING LTD
PI BRISTOL
PA TEMPLE CIRCUS, TEMPLE WAY, BRISTOL BS1 6BE, ENGLAND
SN 1367-2630
J9 NEW J PHYS
JI New J. Phys.
PD OCT 13
PY 2016
VL 18
AR 103018
DI 10.1088/1367-2630/18/10/103018
PG 9
WC Physics, Multidisciplinary
SC Physics
GA EA2NX
UT WOS:000386431600001
ER
PT J
AU Wang, X
Heald, CL
Sedlacek, AJ
de Sa, SS
Martin, ST
Alexander, ML
Watson, TB
Aiken, AC
Springston, SR
Artaxo, P
AF Wang, Xuan
Heald, Colette L.
Sedlacek, Arthur J.
de Sa, Suzane S.
Martin, Scot T.
Alexander, M. Lizabeth
Watson, Thomas B.
Aiken, Allison C.
Springston, Stephen R.
Artaxo, Paulo
TI Deriving brown carbon from multiwavelength absorption measurements:
method and application to AERONET and Aethalometer observations
SO ATMOSPHERIC CHEMISTRY AND PHYSICS
LA English
DT Article
ID AEROSOL LIGHT-ABSORPTION; SOUTHEASTERN UNITED-STATES; FOSSIL-FUEL
COMBUSTION; BLACK CARBON; OPTICAL-PROPERTIES; ORGANIC AEROSOL; ANGSTROM
EXPONENT; CROSS-SECTION; SPECTRAL DEPENDENCE; SOLAR-RADIATION
AB The radiative impact of organic aerosols (OA) is a large source of uncertainty in estimating the global direct radiative effect (DRE) of aerosols. This radiative impact includes not only light scattering but also light absorption from a subclass of OA referred to as brown carbon (BrC). However, the absorption properties of BrC are poorly understood, leading to large uncertainties in modeling studies. To obtain observational constraints from measurements, a simple absorption Angstrom exponent (AAE) method is often used to separate the contribution of BrC absorption from that of black carbon (BC). However, this attribution method is based on assumptions regarding the spectral dependence of BC that are often violated in the ambient atmosphere. Here we develop a new AAE method which improves upon previous approaches by using the information from the wavelength-dependent measurements themselves and by allowing for an atmospherically relevant range of BC properties, rather than fixing these at a single assumed value. We note that constraints on BC optical properties and mixing state would help further improve this method. We apply this method to multiwavelength absorption aerosol optical depth (AAOD) measurements at AERONET sites worldwide and surface aerosol absorption measurements at multiple ambient sites. We estimate that BrC globally contributes up to 40% of the seasonally averaged absorption at 440 nm. We find that the mass absorption coefficient of OA (OA-MAC) is positively correlated with the BC/OA mass ratio. Based on the variability in BC properties and BC/OA emission ratio, we estimate a range of 0.05-1.5 m(2) g(-1) for OA-MAC at 440 nm. Using the combination of AERONET and OMI UV absorption observations we estimate that the AAE(388/440nm) for BrC is generally similar to 4 worldwide, with a smaller value in Europe (<2). Our analyses of observations at two surface sites (Cape Cod, to the southeast of Boston, and the GoAmazon2014/5 T3 site, to the west of Manaus, Brazil) reveal no significant relationship between BrC absorptivity and photochemical aging in urban-influenced conditions. However, the absorption of BrC measured during the biomass burning season near Manaus is found to decrease with photochemical aging with a lifetime of similar to 1 day. This lifetime is comparable to previous observations within a biomass burning plume but much slower than estimated from laboratory studies. Given the large uncertainties associated with AERONET retrievals of AAOD, the most challenging aspect of our analysis is that an accurate, globally distributed, multiple-wavelength aerosol absorption measurement dataset is unavailable at present. Thus, achieving a better understanding of the properties, evolution, and impacts of global BrC will rely on the future deployment of accurate multiple-wavelength absorption measurements to which AAE methods, such as the approach developed here, can be applied.
C1 [Wang, Xuan; Heald, Colette L.] MIT, Dept Civil & Environm Engn, 77 Massachusetts Ave, Cambridge, MA 02139 USA.
[Heald, Colette L.] MIT, Dept Earth Atmospher & Planetary Sci, Cambridge, MA 02139 USA.
[Sedlacek, Arthur J.; Watson, Thomas B.; Springston, Stephen R.] Brookhaven Natl Lab, Environm & Climate Sci Dept, Upton, NY 11973 USA.
[de Sa, Suzane S.; Martin, Scot T.] Harvard Univ, Sch Engn & Appl Sci, Cambridge, MA 02138 USA.
[Alexander, M. Lizabeth] Pacific Northwest Natl Lab, Richard, WA USA.
[Aiken, Allison C.] Los Alamos Natl Lab, Earth & Environm Sci Div, Los Alamos, NM USA.
[Artaxo, Paulo] Univ Sao Paulo, Inst Phys, Sao Paulo, Brazil.
RP Wang, X (reprint author), MIT, Dept Civil & Environm Engn, 77 Massachusetts Ave, Cambridge, MA 02139 USA.
EM xuanw12@mit.edu
RI Aiken, Allison/B-9659-2009; Martin, Scot/G-1094-2015; Artaxo,
Paulo/E-8874-2010
OI Aiken, Allison/0000-0001-5749-7626; Martin, Scot/0000-0002-8996-7554;
Artaxo, Paulo/0000-0001-7754-3036
FU EPA-STAR program; US EPA [RD-83503301]; Office of Biological and
Environmental Research
FX This work was supported by the EPA-STAR program. Although the research
described in this article was funded in part by the US EPA through
grant/cooperative agreement RD-83503301, it has not been subjected to
the EPA's required peer and policy review and therefore does not
necessarily reflect the views of the EPA and no official endorsement
should be inferred. The GoAmazon2014/5 and TCAP data were obtained from
the Atmospheric Radiation Measurement (ARM) Climate Research Facility, a
US Department of Energy Office of Science user facility sponsored by the
Office of Biological and Environmental Research. For the GoAmazon2014/5
data, we also acknowledge the support from the Central Office of the
Large Scale Biosphere Atmosphere Experiment in Amazonia (LBA), the
Instituto Nacional de Pesquisas da Amazonia (INPA), and the Universidade
do Estado do Amazonia (UEA). The work of GoAmazon2014/5 campaign was
conducted under 001030/2012-4 of the Brazilian National Council for
Scientific and Technological Development (CNPq). The AMS measurement at
GoAmazon2014/5-T3 site was performed using EMSL, a DOE Office of Science
User Facility sponsored by the Office of Biological and Environmental
Research and located at Pacific Northwest National Laboratory. We thank
Jesse Kroll, Eleanor Browne, Kelsey Boulanger, Anthony Carasquillo, and
Kelly Daumit for AMS measurement during TCAP. We also thank the
Norwegian Institute for Air Research (NILU) and the NOAA Earth System
Research Laboratory for providing the EMEP and NOAA/ESRL background site
measurements, as well as the AERONET staff for establishing and
maintaining the sun photometer network used in this study.
NR 86
TC 0
Z9 0
U1 18
U2 18
PU COPERNICUS GESELLSCHAFT MBH
PI GOTTINGEN
PA BAHNHOFSALLEE 1E, GOTTINGEN, 37081, GERMANY
SN 1680-7316
EI 1680-7324
J9 ATMOS CHEM PHYS
JI Atmos. Chem. Phys.
PD OCT 13
PY 2016
VL 16
IS 19
BP 12733
EP 12752
DI 10.5194/acp-16-12733-2016
PG 20
WC Meteorology & Atmospheric Sciences
SC Meteorology & Atmospheric Sciences
GA DY8TI
UT WOS:000385403500001
ER
PT J
AU Rao, XL
Dixon, RA
AF Rao, Xiaolan
Dixon, Richard A.
TI The Differences between NAD-ME and NADP-ME Subtypes of C-4
Photosynthesis: More than Decarboxylating Enzymes
SO FRONTIERS IN PLANT SCIENCE
LA English
DT Article
DE C-4 photosynthesis; C-4 plants; NAD-ME subtype; NADP-ME subtype;
comparative transcriptome analysis
ID BUNDLE-SHEATH-CELLS; LEAF DEVELOPMENTAL GRADIENT; MALIC ENZYME;
MESOPHYLL CHLOROPLASTS; FUNCTIONAL-DIFFERENTIATION; COMPARATIVE
PROTEOMICS; USE EFFICIENCY; KRANZ ANATOMY; C4 PLANTS; ZEA-MAYS
AB As an adaptation to changing climatic conditions that caused high rates of photorespiration, C-4 plants have evolved to display higher photosynthetic efficiency than C-3 plants under elevated temperature, high light intensities, and drought. The C-4 plants independently evolved more than 60 times in 19 families of angiosperms to establish similar but not uniform C-4 mechanisms to concentrate CO2 around the carboxylating enzyme Rubisco (ribulose bisphosphate carboxylase oxygenase). C-4 photosynthesis is divided into at least two basic biochemical subtypes based on the primary decarboxylating enzymes, NAD-dependent malic enzyme (NAD-ME) and NADP-dependent malic enzyme (NADP-ME). The multiple polygenetic origins of these subtypes raise questions about the association of C-4 variation between biochemical subtypes and diverse lineages. This review addresses the differences in evolutionary scenario, leaf anatomy, and especially C-4 metabolic flow, C-4 transporters, and cell-specific function deduced from recently reported cell-specific transcriptomic, proteomic, and metabolic analyses of NAD-ME and NADP-ME subtypes. Current omic analysis has revealed the extent to which component abundances differ between the two biochemical subtypes, leading to a better understanding of C-4 photosynthetic mechanisms in NAD-ME and NADP-ME subtypes.
C1 [Rao, Xiaolan; Dixon, Richard A.] Univ North Texas, BioDiscovery Inst, Denton, TX 76203 USA.
[Rao, Xiaolan; Dixon, Richard A.] Univ North Texas, Dept Biol Sci, Denton, TX 76203 USA.
[Rao, Xiaolan; Dixon, Richard A.] US DOE, BioEnergy Sci Ctr, Oak Ridge, TN 37830 USA.
RP Rao, XL; Dixon, RA (reprint author), Univ North Texas, BioDiscovery Inst, Denton, TX 76203 USA.; Rao, XL; Dixon, RA (reprint author), Univ North Texas, Dept Biol Sci, Denton, TX 76203 USA.; Rao, XL; Dixon, RA (reprint author), US DOE, BioEnergy Sci Ctr, Oak Ridge, TN 37830 USA.
EM xiaolan.rao@unt.edu; richard.dixon@unt.edu
FU US Department of Energy Advanced Research Projects Agency-Energy
(ARPA-E); US Department of Energy Bioenergy Sciences Center (BESC),
through the Office of Biological and Environmental Research in the DOE
Office of Science [BER DE-AC05-00OR2727]
FX The research from the authors' laboratory was supported by grants to RD
from both the US Department of Energy Advanced Research Projects
Agency-Energy (ARPA-E) and the US Department of Energy Bioenergy
Sciences Center (BESC, grant # BER DE-AC05-00OR2727), through the Office
of Biological and Environmental Research in the DOE Office of Science.
NR 68
TC 0
Z9 0
U1 14
U2 14
PU FRONTIERS MEDIA SA
PI LAUSANNE
PA PO BOX 110, EPFL INNOVATION PARK, BUILDING I, LAUSANNE, 1015,
SWITZERLAND
SN 1664-462X
J9 FRONT PLANT SCI
JI Front. Plant Sci.
PD OCT 13
PY 2016
VL 7
AR 1525
DI 10.3389/fpls.2016.01525
PG 9
WC Plant Sciences
SC Plant Sciences
GA DY7AO
UT WOS:000385281800001
PM 27790235
ER
PT J
AU Moshammer, K
Jasper, AW
Popolan-Vaida, DM
Wang, ZD
Shankar, VSB
Ruwe, L
Taatjes, CA
Dagaut, P
Hansen, N
AF Moshammer, Kai
Jasper, Ahren W.
Popolan-Vaida, Denisia M.
Wang, Zhandong
Shankar, Vijai Shankar Bhavani
Ruwe, Lena
Taatjes, Craig A.
Dagaut, Philippe
Hansen, Nils
TI Quantification of the Keto-Hydroperoxide (HOOCH2OCHO) and Other Elusive
Intermediates during Low-Temperature Oxidation of Dimethyl Ether
SO JOURNAL OF PHYSICAL CHEMISTRY A
LA English
DT Article
ID PHOTOIONIZATION CROSS-SECTIONS; VALENCE-SHELL PHOTOABSORPTION;
COMBUSTION CHEMISTRY; DISSOCIATIVE PHOTOIONIZATION; MASS-SPECTROMETRY;
ALTERNATIVE FUEL; FLAME CHEMISTRY; N-BUTANE; PHOTODISSOCIATION;
SYNCHROTRON
AB This work provides new temperature-dependent mole fractions of elusive intermediates relevant to the low temperature oxidation of dimethyl ether (DME). It extends the previous study of Moshammer et al. [J. Phys. Chem. A 2015, 119, 7361-7374] in which a combination of a jet-stirred reactor and molecular beam mass spectrometry with single photon ionization via tunable synchrotron-generated vacuum ultraviolet radiation was used to identify (but not quantify) several highly oxygenated species. Here, temperature-dependent concentration profiles of 17 components were determined in the range of 450-1000 K and compared to up-to-date kinetic modeling results. Special emphasis is paid toward the validation and application of a theoretical method for predicting photoionization cross sections that are hard to obtain experimentally but essential to turn mass spectral data into mole fraction profiles. The presented approach enabled the quantification of the hydroperoxymethyl formate (HOOCH2OCH2O), which is a key intermediate in the low-temperature oxidation of DME. The quantification of this keto-hydroperoxide together with the temperature-dependent concentration profiles of other intermediates including H2O2, HCOOH, CH3OCHO, and CH3OOH reveals new opportunities for the development of a next-generation DME combustion chemistry mechanism.
C1 [Moshammer, Kai; Jasper, Ahren W.; Taatjes, Craig A.; Hansen, Nils] Sandia Natl Labs, Combust Res Facil, Livermore, CA 94551 USA.
[Popolan-Vaida, Denisia M.] Univ Calif Berkeley, Dept Chem, Berkeley, CA 94720 USA.
[Popolan-Vaida, Denisia M.] Lawrence Berkeley Natl Lab, Div Chem Sci, Berkeley, CA 94720 USA.
[Wang, Zhandong; Shankar, Vijai Shankar Bhavani] KAUST, CCRC, Thuwal 239556900, Saudi Arabia.
[Ruwe, Lena] Univ Bielefeld, Dept Chem, D-33615 Bielefeld, Germany.
[Dagaut, Philippe] ICARE, CNRS INSIS, F-45071 Orleans 2, France.
[Moshammer, Kai] Phys Tech Bundesanstalt, Bundesallee 100, D-38116 Braunschweig, Germany.
RP Hansen, N (reprint author), Sandia Natl Labs, Combust Res Facil, Livermore, CA 94551 USA.
EM nhansen@sandia.gov
RI Dagaut, Philippe/C-1709-2008; Wang, Zhandong/B-2839-2009; Hansen,
Nils/G-3572-2012
OI Dagaut, Philippe/0000-0003-4825-3288;
FU U.S. Department of Energy (DOE), Office of Science, Office of Basic
Energy Sciences; DOE Gas Phase Chemical Physics Program at Lawrence
Berkeley National Laboratory [DEAC02-05CH11231]; European Research
Council under the European Community's Seventh Framework Programme
(FP7)/ERC [291049-2G-CSafe]; King Abdullah University of Science and
Technology; Office of Science, Office of Basic Energy Sciences, of the
U.S. DOE [DEAC02-05CH11231]; National Nuclear Security Administration
[DE-AC04-94-AL85000]
FX This material is based upon work supported by the U.S. Department of
Energy (DOE), Office of Science, Office of Basic Energy Sciences.
D.M.P.-V. is supported by the DOE Gas Phase Chemical Physics Program at
Lawrence Berkeley National Laboratory, under Contract DEAC02-05CH11231.
We thank Paul Fugazzi for technical assistance and Profs. Leone,
Sarathy, and Kohse-Hoinghaus for continuing support of this project, and
Prof. Lucchese for providing his code. P.D. received funding from the
European Research Council under the European Community's Seventh
Framework Programme (FP7/2007-2013)/ERC Grant Agreement 291049-2G-CSafe.
Z.W. and V.S.B.S. acknowledge competitive research funding given to the
Clean Combustion Research Center from the King Abdullah University of
Science and Technology. The Advanced Light Source is supported by the
Director, Office of Science, Office of Basic Energy Sciences, of the
U.S. DOE under Contract DEAC02-05CH11231. Sandia is a multimission
laboratory operated by Sandia Corporation, a Lockheed Martin Company,
for the National Nuclear Security Administration under Contract
DE-AC04-94-AL85000.
NR 58
TC 0
Z9 0
U1 21
U2 21
PU AMER CHEMICAL SOC
PI WASHINGTON
PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA
SN 1089-5639
J9 J PHYS CHEM A
JI J. Phys. Chem. A
PD OCT 13
PY 2016
VL 120
IS 40
BP 7890
EP 7901
DI 10.1021/acs.jpca.6b06634
PG 12
WC Chemistry, Physical; Physics, Atomic, Molecular & Chemical
SC Chemistry; Physics
GA DZ1OD
UT WOS:000385606800012
ER
PT J
AU Herascu, N
Hunter, MS
Shafiei, G
Najafi, M
Johnson, TW
Fromme, P
Zazubovich, V
AF Herascu, Nicoleta
Hunter, Mark S.
Shafiei, Golia
Najafi, Mehdi
Johnson, T. Wade
Fromme, Petra
Zazubovich, Valter
TI Spectral Hole Burning in Cyanobacterial Photosystem I with P700 in
Oxidized and Neutral States
SO JOURNAL OF PHYSICAL CHEMISTRY B
LA English
DT Article
ID RED ANTENNA STATES; PIGMENT-PROTEIN COMPLEXES; SP PCC 6803;
PHOTOSYNTHETIC PURPLE BACTERIA; SINGLE-MOLECULE SPECTROSCOPY;
SECONDARY-ELECTRON ACCEPTOR; EXCITATION-ENERGY TRANSFER; SYNECHOCYSTIS
SP PCC-6803; SYNECHOCOCCUS-ELONGATUS; LOW-TEMPERATURE
AB We explored the rich satellite hole structures emerging as a result of spectral hole burning in cyanobacterial photosystem I (PSI) and demonstrated that hole burning properties of PSI, particularly at high resolution, are strongly affected by the oxidation state of the primary donor P700, as P700(+) effectively quenches the excitations of the lowest-energy antenna states responsible for fluorescence. Obtaining better control of this variable will be crucial for high-resolution ensemble experiments on protein energy landscapes in PSI. The separate nonphotochemical spectral hole burning (NPHB) signatures of various red antenna states were obtained, allowing for additional constraints on excitonic structure based calculations. Preliminary evidence is presented for an additional red state of PSI of T. elongatus peaked at 712.6 nm, distinct from previously reported C708 and C715 states and possibly involving chlorophyll B15. Excitation at wavelengths as long as 800 rim results in charge separation at cryogenic temperatures in PSI also in Synechacystis sp. PCC 6803. Both the "P700(+) minus P700" holes and nonphotochemical spectral holes were subjected to thermocycling. The distribution-of barriers manifesting in recovery of the "P700(+) minus P700" signature contains two components in sample-dependent proportions, likely reflecting the percentages Of FA and F-B clusters being successfully prereduced before the optical experiment. The barrier distribution for the recovery of the lower-energy nonphotochemical spectral holes resembles those observed for other pigment protein complexes, suggesting similar structural elements are responsible for NPHB. Higher-energy components exhibit evidence of "domino effects" such as shifts of certain bands persisting past the lower-energy hole recovery. Thus, conformational changes triggered by excitation of one pigment likely can affect multiple pigments in this tightly packed-system.
C1 [Herascu, Nicoleta; Shafiei, Golia; Najafi, Mehdi; Zazubovich, Valter] Concordia Univ, Dept Phys, 7141 Sherbrooke St West, Montreal, PQ H4B 1R4, Canada.
[Hunter, Mark S.; Fromme, Petra] Arizona State Univ, Dept Chem & Biochem, Tempe, AZ USA.
[Johnson, T. Wade] Susquehanna Univ, Dept Chem, Selinsgrove, PA USA.
[Hunter, Mark S.] Lawrence Livermore Natl Lab, Livermore, CA 94550 USA.
RP Zazubovich, V (reprint author), Concordia Univ, Dept Phys, 7141 Sherbrooke St West, Montreal, PQ H4B 1R4, Canada.
EM valter.zazubovits@concordia.ca
FU National Science Foundation [MCB-0417142]
FX The Concordia researchers thank NSERC, CFI, and Concordia University.
This work was also supported by the National Science Foundation Grant
No. MCB-0417142 to P.F.
NR 64
TC 0
Z9 0
U1 10
U2 10
PU AMER CHEMICAL SOC
PI WASHINGTON
PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA
SN 1520-6106
J9 J PHYS CHEM B
JI J. Phys. Chem. B
PD OCT 13
PY 2016
VL 120
IS 40
BP 10483
EP 10495
DI 10.1021/acs.jpcb.6b07803
PG 13
WC Chemistry, Physical
SC Chemistry
GA DZ1OC
UT WOS:000385606700007
ER
PT J
AU Pahk, I
Kodis, G
Fleming, GR
Moore, TA
Moore, AL
Gust, D
AF Pahk, Ian
Kodis, Gerdenis
Fleming, Graham R.
Moore, Thomas A.
Moore, Ana L.
Gust, Devens
TI Artificial Photosynthetic Reaction Center Exhibiting Acid-Responsive
Regulation of Photoinduced Charge Separation
SO JOURNAL OF PHYSICAL CHEMISTRY B
LA English
DT Article
ID PHOTOPROTECTIVE ENERGY-DISSIPATION; TIME-RESOLVED FLUORESCENCE;
LIGHT-HARVESTING-COMPLEX; ELECTRON-TRANSFER; PHOTOSYSTEM-II; CHLOROPHYLL
FLUORESCENCE; EXCITATION-ENERGY; ISOLATED-CHLOROPLASTS; SOLVENT
DEPENDENCE; HIGHER-PLANTS
AB Nonphotochemical quenching (NPQ) is a photoprotective regulatory mechanism employed by many photosynthetic organisms to dynamically modulate energy flow within the photosynthetic apparatus in response to fluctuating light conditions. Activated by decreases in lumen pH produced during periods of high photon flux, NPQ induces rapid thermal dissipation of excess excitation energy. As a result, the rate of charge separation (CS) decreases, thereby limiting the accumulation of potentially deleterious reactive intermediates and byproducts. Herein, a molecular triad that functionally mimics the effects of NPQ associated with an artificial photosynthetic reaction center is described. Steady-state absorption and emission, time-resolved fluorescence, and transient absorption spectroscopies have been used to demonstrate a 1 order of magnitude reduction in the CS quantum yield via reversible protonation of an excited-state-quenching molecular switch moiety. As in the natural system, the populations of unquenched and quenched states and therefore the overall yields of CS were found to be dependent on acid concentration.
C1 [Pahk, Ian; Kodis, Gerdenis; Moore, Thomas A.; Moore, Ana L.; Gust, Devens] Arizona State Univ, Sch Mol Sci, Tempe, AZ 85287 USA.
[Fleming, Graham R.] Univ Calif Berkeley, Mol Biophys & Integrated Bioimaging Div, Lawrence Berkeley Natl Lab, Berkeley, CA 94720 USA.
[Fleming, Graham R.] Univ Calif Berkeley, Dept Chem, Berkeley, CA 94720 USA.
[Fleming, Graham R.] Univ Calif Berkeley, Inst QB3, Berkeley, CA 94720 USA.
RP Moore, TA; Moore, AL; Gust, D (reprint author), Arizona State Univ, Sch Mol Sci, Tempe, AZ 85287 USA.
EM tmoore@asu.edu; amoore@asu.edu; gust@asu.edu
FU Office of Basic Energy Sciences, Division of Chemical Sciences,
Geosciences, and Energy Biosciences, Department of Energy
[DE-FG02-03ER15393]; Office of Basic Energy Sciences, Division of
Chemical Sciences, Geosciences, and Energy Biosciences of the US
Department of Energy [DE-AC02-05CH11231, DE-AC-03-76F000098]
FX We thank Kul Bhushan for the preparation of some materials used while
developing methodology for these experiments. This work was supported by
the Office of Basic Energy Sciences, Division of Chemical Sciences,
Geosciences, and Energy Biosciences, Department of Energy, under
contract DE-FG02-03ER15393. Graham R. Fleming's contribution was
supported by the Office of Basic Energy Sciences, Division of Chemical
Sciences, Geosciences, and Energy Biosciences of the US Department of
Energy under contract DE-AC02-05CH11231 and through grant
DE-AC-03-76F000098.
NR 43
TC 0
Z9 0
U1 8
U2 8
PU AMER CHEMICAL SOC
PI WASHINGTON
PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA
SN 1520-6106
J9 J PHYS CHEM B
JI J. Phys. Chem. B
PD OCT 13
PY 2016
VL 120
IS 40
BP 10553
EP 10562
DI 10.1021/acs.jpcb.6b07609
PG 10
WC Chemistry, Physical
SC Chemistry
GA DZ1OC
UT WOS:000385606700015
ER
PT J
AU Chang, TM
Xantheas, SS
Vasdekis, AE
AF Chang, Tsun-Mei
Xantheas, Sotiris S.
Vasdekis, Andreas E.
TI Mesoscale Polymer Dissolution Probed by Raman Spectroscopy and Molecular
Simulations
SO JOURNAL OF PHYSICAL CHEMISTRY B
LA English
DT Article
ID IMMERSION IMPRINT LITHOGRAPHY; PARTICLE MESH EWALD; FORCE-FIELD;
DYNAMICS; DIFFUSION; MODEL; PHOTOLITHOGRAPHY; PARAMETERS; LANGEVIN;
SYSTEMS
AB The diffusion of various solvents into a polystyrene (PS) matrix was probed experimentally by monitoring the temporal profiles of the Raman spectra and theoretically from molecular dynamics simulations. The simulation results assist in providing a fundamental, molecular-level connection between the mixing/dissolution processes and the difference, Delta delta = delta(solvent) - delta(PS), in the values of the Hildebrand parameter (delta) between the two components of the binary systems: solvents having values of delta similar to those for PS (small Delta delta) exhibit fast diffusion into the polymer matrix, whereas the diffusion slows down considerably when the delta s are different (large Delta delta). To this end, the Hildebrand parameter was identified as a useful descriptor that governs the process of mixing in polymer-solvent binary systems. The experiments also provide insight into further refinements of the models specific to non-Fickian diffusion phenomena that need to be used in the simulations.
C1 [Chang, Tsun-Mei] Univ Wisconsin Parkside, POB 2000, Kenosha, WI 53141 USA.
[Xantheas, Sotiris S.] Pacific Northwest Natl Lab, Div Phys Sci, 902 Battelle Blvd,POB 999,MS K1-83, Richland, WA 99352 USA.
[Vasdekis, Andreas E.] Pacific Northwest Natl Lab, Environm Mol Sci Lab, POB 999, Richland, WA 99352 USA.
[Vasdekis, Andreas E.] Univ Idaho, Dept Phys, Moscow, ID 83844 USA.
RP Xantheas, SS (reprint author), Pacific Northwest Natl Lab, Div Phys Sci, 902 Battelle Blvd,POB 999,MS K1-83, Richland, WA 99352 USA.; Vasdekis, AE (reprint author), Pacific Northwest Natl Lab, Environm Mol Sci Lab, POB 999, Richland, WA 99352 USA.; Vasdekis, AE (reprint author), Univ Idaho, Dept Phys, Moscow, ID 83844 USA.
EM sotiris.xantheas@pnnl.gov; andreasv@uidaho.edu
OI Xantheas, Sotiris/0000-0002-6303-1037
FU US Department of Energy, Office of Science, Office of Basic Energy
Sciences, Division of Chemical Sciences, Geosciences and Biosciences;
Office of Science of the U.S. Department of Energy [DE-AC02-05CH11231];
INBRE program [P20 GM103408]; National Institutes of Health (NIH);
Pacific Northwest National Laboratory (Linus Pauling Fellowship)
[PN12005/2406]; Department of Energy's Office of Biological and
Environmental Research located at Pacific Northwest National Laboratory
FX S.S.X. was supported by the US Department of Energy, Office of Science,
Office of Basic Energy Sciences, Division of Chemical Sciences,
Geosciences and Biosciences. Pacific Northwest National Laboratory
(PNNL) is a multiprogram national laboratory operated for DOE by
Battelle. This research also used resources of the National Energy
Research Scientific Computing Center, which is supported by the Office
of Science of the U.S. Department of Energy under Contract No.
DE-AC02-05CH11231. A.E.V. acknowledges funding from the INBRE program
(Project ID: P20 GM103408), the National Institutes of Health (NIH), and
the Pacific Northwest National Laboratory (Linus Pauling Fellowship -
PN12005/2406). Part of the research was performed at EMSL, a national
user facility sponsored by the Department of Energy's Office of
Biological and Environmental Research located at Pacific Northwest
National Laboratory.
NR 35
TC 0
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U1 4
U2 4
PU AMER CHEMICAL SOC
PI WASHINGTON
PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA
SN 1520-6106
J9 J PHYS CHEM B
JI J. Phys. Chem. B
PD OCT 13
PY 2016
VL 120
IS 40
BP 10581
EP 10587
DI 10.1021/acs.jpcb.6b05565
PG 7
WC Chemistry, Physical
SC Chemistry
GA DZ1OC
UT WOS:000385606700018
PM 27653929
ER
PT J
AU Song, WT
Leung, K
Shao, Q
Gaskell, KJ
Reutt-Robey, JE
AF Song, Wentao
Leung, Kevin
Shao, Qian
Gaskell, Karen J.
Reutt-Robey, Janice E.
TI Complexation and Phase Evolution at Dimethylformamide-Ag(111) Interfaces
SO JOURNAL OF PHYSICAL CHEMISTRY C
LA English
DT Article
ID TOTAL-ENERGY CALCULATIONS; WAVE BASIS-SET; COORDINATION CHEMISTRY;
METAL-SURFACES; N,N-DIMETHYLFORMAMIDE; NETWORKS; AG(111); ATOM
AB The interaction of solvent molecules with metallic surfaces impacts many interfacial chemical processes: We investigate the chemical and structure evolution that follows adsorption of the polar solvent dimethylformamide (DIM) on Ag(111). An Ag(DMF)(2) coordination complex forms spontaneously by DMF etching of Ag(111), yielding Allied films of the complexes and DMF. Utilizing ultrahigh vacuum scanning tunneling microscopy (UHV-STM), in combination with X-ray photoelectron spectroscopy (XPS) and density functional theory (DFT) computations, we map monolayer phases from the 2-D gas regime, consisting of a binary mixture of DMF and Ag(DMF)(2), through the saturation monolayer limit, in which these two chemical species phase separate into ordered islands. Structural models for the near-square DMF phase and the chain-like Ag(DMF)(2) phase are presented and supported by DFT computation. Interface evolution is summarized in a surface pressure-composition phase diagram, which allows structure prediction over arbitrary experimental conditions. This work reveals new surface coordination chemistry for an important electrolyte electrode system and illustrates how surface pressure can be used to tune monolayer phases.
C1 [Song, Wentao; Shao, Qian; Gaskell, Karen J.; Reutt-Robey, Janice E.] Univ Maryland, Dept Chem & Biochem, College Pk, MD 20742 USA.
[Leung, Kevin] Sandia Natl Labs, POB 5800, Albuquerque, NM 87185 USA.
RP Reutt-Robey, JE (reprint author), Univ Maryland, Dept Chem & Biochem, College Pk, MD 20742 USA.
EM rrobey@umd.edu
FU U.S. Department of Energy's National Nuclear Security Administration
[DE-AC04-94AL85000]; Nanostructures for Electrical Energy Storage
(NEES), an Energy Frontier Research Center - U.S. Department of Energy,
Office of Science, Basic Energy Sciences [DESC0001160]; National Science
Foundation (NSF) [CHE-1310380]
FX The author would like to thank Dr. Yilin Wang and Mr. Jonathan Larson
for useful discussions. Sandia National Laboratories is a multiprogram
laboratory managed and operated by Sandia Corporation, a wholly owned
subsidiary of Lockheed Martin Corporation, for the U.S. Department of
Energy's National Nuclear Security Administration under Contract
DE-AC04-94AL85000. Aspects of this work was supported as part of the
Nanostructures for Electrical Energy Storage (NEES), an Energy Frontier
Research Center funded by the U.S. Department of Energy, Office of
Science, Basic Energy Sciences under Award Number DESC0001160. Portions
of this work is based on research supported by the National Science
Foundation (NSF) under Grant No. CHE-1310380.
NR 42
TC 0
Z9 0
U1 7
U2 7
PU AMER CHEMICAL SOC
PI WASHINGTON
PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA
SN 1932-7447
J9 J PHYS CHEM C
JI J. Phys. Chem. C
PD OCT 13
PY 2016
VL 120
IS 40
BP 22979
EP 22988
DI 10.1021/acs.jpcc.6b06870
PG 10
WC Chemistry, Physical; Nanoscience & Nanotechnology; Materials Science,
Multidisciplinary
SC Chemistry; Science & Technology - Other Topics; Materials Science
GA DZ1OF
UT WOS:000385607000024
ER
PT J
AU Loheac, A
Barbour, A
Komanicky, V
Zhu, CH
Collini, J
Ruffino, A
Liu, YH
You, H
Pierce, MS
AF Loheac, Andrew
Barbour, Andi
Komanicky, Vladimir
Zhu, Chenhui
Collini, John
Ruffino, Anthony
Liu, Yihua
You, Hoydoo
Pierce, Michael S.
TI Interaction of Molecular Oxygen with a Hexagonally Reconstructed Au(001)
Surface
SO JOURNAL OF PHYSICAL CHEMISTRY C
LA English
DT Article
ID X-RAY REFLECTIVITY; SCANNING-TUNNELING-MICROSCOPY; ELEVATED PRESSURES;
AU(100) SURFACE; AU(111) SURFACE; GOLD SURFACES; AU SURFACES;
ADSORPTION; CHEMISORPTION; SIZE
AB Kinetics of molecular oxygen/Au(001) surface interaction has been studied at high temperature and near atmospheric pressures of O-2 gas with in situ X-ray scattering measurements. We find that the hexagonal reconstruction (hex) of Au(001) surface lifts to (1 x 1) in the presence of 02 gas, indicating that the (1 x 1) is more favored when some oxygen atoms present on the surface. The measured lifting rate constant vs temperature is found to be highest at intermediate temperature exhibiting a "volcano"-type behavior. At low temperature, the hex-to-(1 x 1) activation barrier (E-act = 1.3(3) eV) limits the lifting. At high temperature, oxygen adsorption energy (E-ads = 1.6(2) eV) limits the lifting. The (1 x 1)-to-hex activation barrier(E-hex = 0.41(14) eV) is also obtained from hex recovery kinetics. The pressure-temperature (PT) surface phase diagram obtained in this study show's three regions: hex at low P and T, (1 x 1) at high P and T, and coexistence of the hex and (1 x 1) at the intermediate P and T.
C1 [Loheac, Andrew; Collini, John; Ruffino, Anthony; Pierce, Michael S.] Rochester Inst Technol, Sch Phys & Astron, Rochester, NY 14623 USA.
[Barbour, Andi; Zhu, Chenhui; Liu, Yihua; You, Hoydoo] Argonne Natl Lab, Div Mat Sci, 9700 S Cass Ave, Argonne, IL 60439 USA.
[Komanicky, Vladimir] Safarik Univ, Fac Sci, Kosice, Slovakia.
[Barbour, Andi] Brookhaven Natl Lab, Upton, NY 11973 USA.
[Zhu, Chenhui] Lawrence Berkeley Natl Lab, Berkeley, CA 94720 USA.
RP Pierce, MS (reprint author), Rochester Inst Technol, Sch Phys & Astron, Rochester, NY 14623 USA.; You, H (reprint author), Argonne Natl Lab, Div Mat Sci, 9700 S Cass Ave, Argonne, IL 60439 USA.
EM hyou@anl.gov; mspsps@rit.edu
FU U.S. Department of Energy (DOE), Office of Basic Energy Sciences (BES),
Materials Sciences and Engineering Division; DOE BES Scientific User
Facilities Division [DE-AC02-06CH11357]; European Regional Development
Fund [ITMS 26220120047]; Research Corporation for Science Advancement
(RCSA) through a Cottrell College Science Award
FX The authors are grateful for the valuable on-site assistance during the
experiments provided by Dr. Evguenia Karapetrova and Dr. Christian
Schlepuetz. The work at Argonne National Laboratory was supported by the
U.S. Department of Energy (DOE), Office of Basic Energy Sciences (BES),
Materials Sciences and Engineering Division, and the use of the Advanced
Photon Source by DOE BES Scientific User Facilities Division, under
Contract No. DE-AC02-06CH11357. The work at Safarik University was
supported by the European Regional Development Fund under Grant No. ITMS
26220120047. The work at RIT was supported by the Research Corporation
for Science Advancement (RCSA) through a Cottrell College Science Award,
and data reduction and image processing was performed using the RIT
Research Computing facilities.
NR 42
TC 0
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U1 5
U2 5
PU AMER CHEMICAL SOC
PI WASHINGTON
PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA
SN 1932-7447
J9 J PHYS CHEM C
JI J. Phys. Chem. C
PD OCT 13
PY 2016
VL 120
IS 40
BP 23001
EP 23008
DI 10.1021/acs.jpcc.6b07020
PG 8
WC Chemistry, Physical; Nanoscience & Nanotechnology; Materials Science,
Multidisciplinary
SC Chemistry; Science & Technology - Other Topics; Materials Science
GA DZ1OF
UT WOS:000385607000026
ER
PT J
AU Wan, C
Hu, MY
Jaegers, NR
Shi, DC
Wang, HM
Gao, F
Qin, ZH
Wang, Y
Hui, JZ
AF Wan, Chuan
Hu, Mary Y.
Jaegers, Nicholas R.
Shi, Dachuan
Wang, Huamin
Gao, Feng
Qin, Zhaohai
Wang, Yong
Hui, Jian Zhi
TI Investigating the Surface Structure of gamma-Al2O3 Supported WOx
Catalysts by High Field Al-27 MAS NMR and Electronic Structure
Calculations
SO JOURNAL OF PHYSICAL CHEMISTRY C
LA English
DT Article
ID GAMMA-ALUMINA SURFACES; SOLID-STATE NMR; DENSITY-FUNCTIONAL THEORY;
ANGLE-SPINNING NMR; TRANSITIONAL ALUMINAS; TUNGSTEN-OXIDE; SITES;
DEHYDRATION; DEPOSITION; TENSORS
AB The metal-support interaction in gamma-Al2O3 supported WOX catalysts is investigated by a combination of high field quantitative single pulse (SP) Al-27 MAS NMR spectroscopy, 2D MQMAS, H-1(27)-Al CP/MAS, and electronic structure calculations. NMR allows the observation of at least seven different Al sites, including a pentahedral Al site (Al-P), three different tetrahedral Al sites (Al-T), and three octahedral Al sites (Al-O). It is found that the AlP site density decreases monotonically with an increased WOX loading, the Al-O site density increases concurrently, and the density of AlT sites remains constant. This suggests that the Al-P sites are the preferred surface anchoring positions for the WOX species. Importantly, the Al-P site isotropic chemical shift observed for the unsupported gamma-Al2O3 at about 38 ppm migrates to the octahedral region with a new isotropic chemical shift value appearing near 7 ppm when the Al-P site is anchored by WOX species. Density functional theory (DFT) computational modeling of the NMR parameters on proposed WOX/gamma-Al2O3 cluster models is carried out to accurately interpret the dramatic chemical shift changes from which the detailed anchoring mechanisms are obtained. It is found that tungsten dimers and monomers are the preferred supported surface species on gamma-Al2O3, wherein one monomeric and several dimeric structures are identified as the most likely surface anchoring structures.
C1 [Wan, Chuan; Hu, Mary Y.; Jaegers, Nicholas R.; Shi, Dachuan; Wang, Huamin; Gao, Feng; Hui, Jian Zhi] Pacific Northwest Natl Lab, Richland, WA 99354 USA.
[Wan, Chuan; Qin, Zhaohai] China Agr Univ, Coll Sci, Beijing 100193, Peoples R China.
[Jaegers, Nicholas R.; Wang, Yong] Washington State Univ, Voiland Sch Chem Engn & Bioengn, Pullman, WA 99163 USA.
RP Hui, JZ (reprint author), Pacific Northwest Natl Lab, Richland, WA 99354 USA.
EM Jianzhi.Hu@pnnl.gov
RI Wan, Chuan/I-4657-2016
OI Wan, Chuan/0000-0002-8226-7619
FU U.S. Department of Energy (DOE), Office of Basic Energy Sciences,
Division of Chemical Sciences, Biosciences and Geosciences
[DE-AC05-RL01830, FWP-47319]; Battelle Memorial Institute [DE-AC06-76RLO
1830]; DOE's Office of Biological and Environmental Research
FX This research was supported by the U.S. Department of Energy (DOE),
Office of Basic Energy Sciences, Division of Chemical Sciences,
Biosciences and Geosciences (DE-AC05-RL01830, FWP-47319). All of the NMR
experiments were performed in the Environmental Molecular Sciences
Laboratory, a national scientific user facility sponsored by the DOE's
Office of Biological and Environmental Research, and located at Pacific
Northwest National Laboratory (PNNL). PNNL is a multiprogram national
laboratory operated for the DOE by Battelle Memorial Institute under
Contract DE-AC06-76RLO 1830.
NR 64
TC 0
Z9 0
U1 24
U2 24
PU AMER CHEMICAL SOC
PI WASHINGTON
PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA
SN 1932-7447
J9 J PHYS CHEM C
JI J. Phys. Chem. C
PD OCT 13
PY 2016
VL 120
IS 40
BP 23093
EP 23103
DI 10.1021/acs.jpcc.6b09060
PG 11
WC Chemistry, Physical; Nanoscience & Nanotechnology; Materials Science,
Multidisciplinary
SC Chemistry; Science & Technology - Other Topics; Materials Science
GA DZ1OF
UT WOS:000385607000036
ER
PT J
AU Owczarek, M
Hujsak, KA
Ferris, DP
Prokofjevs, A
Majerz, I
Szklarz, P
Zhang, HC
Sarjeant, AA
Stern, CL
Jakubas, R
Hong, S
Dravid, VP
Stoddart, JF
AF Owczarek, Magdalena
Hujsak, Karl A.
Ferris, Daniel P.
Prokofjevs, Aleksandrs
Majerz, Irena
Szklarz, Przemyslaw
Zhang, Huacheng
Sarjeant, Amy A.
Stern, Charlotte L.
Jakubas, Ryszard
Hong, Seungbum
Dravid, Vinayak P.
Stoddart, J. Fraser
TI Flexible ferroelectric organic crystals
SO NATURE COMMUNICATIONS
LA English
DT Article
ID ROOM-TEMPERATURE FERROELECTRICITY; CAMBRIDGE STRUCTURAL DATABASE;
DOT-HALOGEN INTERACTIONS; DIISOPROPYLAMMONIUM BROMIDE
AB Flexible organic materials possessing useful electrical properties, such as ferroelectricity, are of crucial importance in the engineering of electronic devices. Up until now, however, only ferroelectric polymers have intrinsically met this flexibility requirement, leaving small-molecule organic ferroelectrics with room for improvement. Since both flexibility and ferroelectricity are rare properties on their own, combining them in one crystalline organic material is challenging. Herein, we report that trisubstituted haloimidazoles not only display ferroelectricity and piezoelectricity-the properties that originate from their non-centrosymmetric crystal lattice-but also lend their crystalline mechanical properties to fine-tuning in a controllable manner by disrupting the weak halogen bonds between the molecules. This element of control makes it possible to deliver another unique and highly desirable property, namely crystal flexibility. Moreover, the electrical properties are maintained in the flexible crystals.
C1 [Owczarek, Magdalena; Ferris, Daniel P.; Prokofjevs, Aleksandrs; Zhang, Huacheng; Sarjeant, Amy A.; Stern, Charlotte L.; Stoddart, J. Fraser] Northwestern Univ, Dept Chem, 2145 Sheridan Rd, Evanston, IL 60208 USA.
[Hujsak, Karl A.; Dravid, Vinayak P.] Northwestern Univ, Dept Mat Sci & Engn, 2170 Campus Dr, Evanston, IL 60208 USA.
[Majerz, Irena] Wroclaw Med Univ, Fac Pharm, Dept Analyt Chem, Borowska 211a, PL-50556 Wroclaw, Poland.
[Szklarz, Przemyslaw; Jakubas, Ryszard] Univ Wroclaw, Fac Chem, F Joliot Curie 14, PL-50383 Wroclaw, Poland.
[Hong, Seungbum] Argonne Natl Lab, Div Mat Sci, 9700 S Cass Ave, Argonne, IL 60439 USA.
[Hong, Seungbum] Korea Adv Inst Sci & Technol, Dept Mat Sci & Engn, Daejeon 34141, South Korea.
RP Stoddart, JF (reprint author), Northwestern Univ, Dept Chem, 2145 Sheridan Rd, Evanston, IL 60208 USA.; Dravid, VP (reprint author), Northwestern Univ, Dept Mat Sci & Engn, 2170 Campus Dr, Evanston, IL 60208 USA.; Hong, S (reprint author), Argonne Natl Lab, Div Mat Sci, 9700 S Cass Ave, Argonne, IL 60439 USA.; Hong, S (reprint author), Korea Adv Inst Sci & Technol, Dept Mat Sci & Engn, Daejeon 34141, South Korea.
EM hong@anl.gov; v-dravid@northwestern.edu; stoddart@northwestern.edu
RI Hong, Seungbum/B-7708-2009
OI Hong, Seungbum/0000-0002-2667-1983
FU Soft and Hybrid Nanotechnology Experimental (SHyNE) Resource [NSF
NNCI-1542205]; MRSEC program at the Materials Research Center [NSF
DMR-1121262]; International Institute for Nanotechnology (IIN); Keck
Foundation; State of Illinois, through the IIN; U.S. Department of
Energy (DOE), Office of Science, Office of Basic Energy Sciences (BES),
Division of Materials Sciences and Engineering
FX This research (project no. 3) was conducted as part of the Joint Center
of Excellence in Integrated Nanosystems (JCIN) at King Abdullaziz City
for Science and Technology (KACST) and Northwestern University. We would
like to thank both KACST and Northwestern University (NU) for their
continued support of this research. The Integrated Molecular Structure
Education and Research Center (IMSERC) at NU is acknowledged for the use
of their facilities. This work made use of the EPIC facility of the
NUANCE Center at Northwestern University, which has received support
from the Soft and Hybrid Nanotechnology Experimental (SHyNE) Resource
(NSF NNCI-1542205); the MRSEC program (NSF DMR-1121262) at the Materials
Research Center; the International Institute for Nanotechnology (IIN);
the Keck Foundation; and the State of Illinois, through the IIN. Work at
Argonne (S. H., PFM imaging/hysteresis loop measurement and analysis)
was supported by the U.S. Department of Energy (DOE), Office of Science,
Office of Basic Energy Sciences (BES), Division of Materials Sciences
and Engineering. We thank the Wroclaw Center for Networking and
Supercomputing for the computer time.
NR 41
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PI LONDON
PA MACMILLAN BUILDING, 4 CRINAN ST, LONDON N1 9XW, ENGLAND
SN 2041-1723
J9 NAT COMMUN
JI Nat. Commun.
PD OCT 13
PY 2016
VL 7
AR 13108
DI 10.1038/ncomms13108
PG 10
WC Multidisciplinary Sciences
SC Science & Technology - Other Topics
GA DZ0QM
UT WOS:000385544800001
PM 27734829
ER
PT J
AU Schenke, B
Schlichting, S
AF Schenke, Bjorn
Schlichting, Soren
TI 3D glasma initial state for relativistic heavy ion collisions
SO PHYSICAL REVIEW C
LA English
DT Article
ID RENORMALIZATION-GROUP; NUCLEAR COLLISIONS; GLUON PRODUCTION;
HIGH-ENERGIES; HERA DATA; SMALL-X; EVOLUTION; CONDENSATE; EQUATION;
MODEL
AB We extend the impact-parameter-dependent Glasma model to three dimensions using explicit small-x evolution of the two incoming nuclear gluon distributions. We compute rapidity distributions of produced gluons and the early-time energy momentum tensor as a function of space-time rapidity and transverse coordinates. We study rapidity correlations and fluctuations of the initial geometry and multiplicity distributions and make comparisons to existing models for the three-dimensional initial state.
C1 [Schenke, Bjorn; Schlichting, Soren] Brookhaven Natl Lab, Dept Phys, Upton, NY 11973 USA.
RP Schenke, B (reprint author), Brookhaven Natl Lab, Dept Phys, Upton, NY 11973 USA.
FU DOE [DE-SC0012704]; Office of Science of the U.S. Department of Energy
[DE-AC02-05CH11231]; DOE Office of Science Early Career Award; Goldhaber
Distinguished Fellowship from Brookhaven Science Associates
FX We thank Piotr Bozek, Wojciech Broniowski, Tuomas Lappi, Long-Gang Pang,
Prithwish Tribedy, and Raju Venugopalan for valuable discussions. B.P.S.
and S.S. are supported under DOE Contract No. DE-SC0012704. This
research used resources of the National Energy Research Scientific
Computing Center, which is supported by the Office of Science of the
U.S. Department of Energy under Contract No. DE-AC02-05CH11231. B.P.S.
acknowledges support from a DOE Office of Science Early Career Award.
S.S. gratefully acknowledges support from a Goldhaber Distinguished
Fellowship from Brookhaven Science Associates.
NR 78
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U1 0
U2 0
PU AMER PHYSICAL SOC
PI COLLEGE PK
PA ONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA
SN 2469-9985
EI 2469-9993
J9 PHYS REV C
JI Phys. Rev. C
PD OCT 13
PY 2016
VL 94
IS 4
AR 044907
DI 10.1103/PhysRevC.94.044907
PG 11
WC Physics, Nuclear
SC Physics
GA DZ1VW
UT WOS:000385630600003
ER
PT J
AU Mookherjee, M
Mainprice, D
Maheshwari, K
Heinonen, O
Patel, D
Hariharan, A
AF Mookherjee, Mainak
Mainprice, David
Maheshwari, Ketan
Heinonen, Olle
Patel, Dhenu
Hariharan, Anant
TI Pressure induced elastic softening in framework aluminosilicate-albite
(NaAlSi3O8)
SO SCIENTIFIC REPORTS
LA English
DT Article
ID GENERALIZED GRADIENT APPROXIMATION; TOTAL-ENERGY CALCULATIONS; WAVE
BASIS-SET; AB-INITIO; ALPHA-QUARTZ; PLAGIOCLASE FELDSPARS;
PHYSICAL-PROPERTIES; CONTINENTAL-CRUST; PHASE-EQUILIBRIA; MANTLE
MINERALS
AB Albite (NaAlSi3O8) is an aluminosilicate mineral. Its crystal structure consists of 3-D framework of Al and Si tetrahedral units. We have used Density Functional Theory to investigate the high-pressure behavior of the crystal structure and how it affects the elasticity of albite. Our results indicate elastic softening between 6-8 GPa. This is observed in all the individual elastic stiffness components. Our analysis indicates that the softening is due to the response of the three-dimensional tetrahedral framework, in particular by the pressure dependent changes in the tetrahedral tilts. At pressure < 6 GPa, the PAW-GGA can be described by a Birch-Murnaghan equation of state with V-0(GGA) = 687.4 angstrom(3), K-0(GGA) = 51.7 GPa, and K-0'(GGA) = 4.7. The shear modulus and its pressure derivative are G(0)(GGA) = 33.7 GPa, and G(0)'(GGA) = 2.9. At 1 bar, the azimuthal compressional and shear wave anisotropy AV(P)(GGA) = 42.8%, and AV(S)(GGA) = 50.1%. We also investigate the densification of albite to a mixture of jadeite and quartz. The transformation is likely to cause a discontinuity in density, compressional, and shear wave velocity across the crust and mantle. This could partially account for the Mohorovicic discontinuity in thickened continental crustal regions.
C1 [Mookherjee, Mainak; Patel, Dhenu] Florida State Univ, Earth Ocean & Atmospher Sci, Earth Mat Lab, Tallahassee, FL 32310 USA.
[Mainprice, David] Univ Montpellier, Geosci Montpellier UMR CNRS 5243, F-34095 Montpellier, France.
[Maheshwari, Ketan] Univ Pittsburgh, Ctr Simulat & Modeling, Pittsburgh, PA 15260 USA.
[Heinonen, Olle] Argonne Natl Lab, Div Mat Sci, 9700 S Cass Ave, Argonne, IL 60439 USA.
[Hariharan, Anant] Cornell Univ, Earth & Atmospher Sci, Ithaca, NY 14850 USA.
RP Mookherjee, M (reprint author), Florida State Univ, Earth Ocean & Atmospher Sci, Earth Mat Lab, Tallahassee, FL 32310 USA.
EM mmookherjee@fsu.edu
RI Mookherjee, Mainak/F-7949-2010
OI Mookherjee, Mainak/0000-0002-0605-5964
FU US-NSF [EAR-1634422]; US DOE, Office of Science [DE-AC02-06CH11357]
FX M.M. is currently supported by US-NSF EAR-1634422. M.M. and K.M.
acknowledges computing resources from ALCF Mira Supercomputer through
grant "ElasticEarthCrust". The work by O.H. was supported in part by the
US DOE, Office of Science under Contract No. DE-AC02-06CH11357. Authors
thank the reviewers and associate editor for their constructive
criticism that helped to enhance the clarity of the manuscript.
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PI LONDON
PA MACMILLAN BUILDING, 4 CRINAN ST, LONDON N1 9XW, ENGLAND
SN 2045-2322
J9 SCI REP-UK
JI Sci Rep
PD OCT 13
PY 2016
VL 6
AR 34815
DI 10.1038/srep34815
PG 10
WC Multidisciplinary Sciences
SC Science & Technology - Other Topics
GA DY9OF
UT WOS:000385463000001
PM 27734903
ER
PT J
AU Anderson, IS
Andreani, C
Carpenter, JM
Festa, G
Gorini, G
Loong, CK
Senesi, R
AF Anderson, I. S.
Andreani, C.
Carpenter, J. M.
Festa, G.
Gorini, G.
Loong, C-K.
Senesi, R.
TI Research opportunities with compact accelerator-driven neutron sources
SO PHYSICS REPORTS-REVIEW SECTION OF PHYSICS LETTERS
LA English
DT Review
DE Compact neutron sources; Neutronics; Accelerator; Nuclear reactions;
Neutron scattering neutron interrogation; Cultural heritage; Detectors
ID NUCLEAR-DATA; CAPTURE THERAPY; NEXT-GENERATION; DETECTOR; ENERGY;
TRANSMISSION; SPALLATION; SYSTEM; SPECTROSCOPY; RADIOGRAPHY
AB Since the discovery of the neutron in 1932 neutron beams have been used in a very broad range of applications, As an aging fleet of nuclear reactor sources is retired the use of compact accelerator-driven neutron sources (CANS) is becoming more prevalent. CANS are playing a significant and expanding role in research and development in science and engineering, as well as in education and training. In the realm of multidisciplinary applications, CANS offer opportunities over a wide range of technical utilization, from interrogation of civil structures to medical therapy to cultural heritage study. This paper aims to provide the first comprehensive overview of the history, current status of operation, and ongoing development of CANS worldwide. The basic physics and engineering regarding neutron production by accelerators, target-moderator systems, and beam line instrumentation are introduced, followed by an extensive discussion of various evolving applications currently exploited at CANS. (C) 2016 Elsevier B.V. All rights reserved.
C1 [Anderson, I. S.] Oak Ridge Natl Lab, Oak Ridge, TN USA.
[Andreani, C.; Festa, G.; Senesi, R.] Univ Roma Tor Vergata, Dept Phys, Via Ric Sci 1, I-00133 Rome, Italy.
[Andreani, C.; Festa, G.; Loong, C-K.; Senesi, R.] Univ Roma Tor Vergata, NAST Ctr, Via Ric Sci 1, I-00133 Rome, Italy.
[Andreani, C.; Senesi, R.] CNR IPCF Sez Messina, Messina, Italy.
[Andreani, C.; Festa, G.; Senesi, R.] Museo Stor Fis, Rome, Italy.
[Andreani, C.; Festa, G.; Senesi, R.] Ctro Studi & Ric Enrico Fermi, Rome, Italy.
[Carpenter, J. M.] Argonne Natl Lab, 9700 S Cass Ave, Argonne, IL 60439 USA.
[Gorini, G.] Univ Milano Bicocca, Milan, Italy.
RP Andreani, C; Festa, G (reprint author), Univ Roma Tor Vergata, Dept Phys, Via Ric Sci 1, I-00133 Rome, Italy.; Andreani, C; Festa, G (reprint author), Univ Roma Tor Vergata, NAST Ctr, Via Ric Sci 1, I-00133 Rome, Italy.
EM carla.andreani@uniroma2.it; giulia.festa@uniroma2.it
RI Gorini, Giuseppe/H-9595-2016
OI Gorini, Giuseppe/0000-0002-4673-0901
FU CNR-STFC
FX This work was partially supported within the CNR-STFC Agreement
(2014-2020) concerning collaboration in scientific research at the ISIS
spallation neutron source. We thank T. Bruckel, B. Galnander, R.
Granada, T. Gutberlet, A. Junghans, Y. Kiyanagi, K. R. Kim, P. Mastinu,
C. Massimi, E. Passoth, M. Pillon, A. Prokofiev, U. Ratzinger, P.
Schillebeeckx, F. Sordo Balbin, M. Uesaka, X. Wang, and J. Wyss, for
providing updated information on the parameters, drawings, and images,
of the CANS described in this work. We are grateful to C.D. Frost for
providing updated information on the ChipIr beam line at ISIS.
NR 156
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U2 12
PU ELSEVIER SCIENCE BV
PI AMSTERDAM
PA PO BOX 211, 1000 AE AMSTERDAM, NETHERLANDS
SN 0370-1573
EI 1873-6270
J9 PHYS REP
JI Phys. Rep.-Rev. Sec. Phys. Lett.
PD OCT 13
PY 2016
VL 654
BP 1
EP 58
DI 10.1016/j.physrep.2016.07.007
PG 58
WC Physics, Multidisciplinary
SC Physics
GA DY1MM
UT WOS:000384859100001
ER
PT J
AU Khachatryan, V
Sirunyan, AM
Tumasyan, A
Adam, W
Asilar, E
Bergauer, T
Brandstetter, J
Brondolin, E
Dragicevic, M
Ero, J
Flechl, M
Friedl, M
Fruhwirth, R
Ghete, VM
Hartl, C
Hormann, N
Hrubec, J
Jeitler, M
Konig, A
Krammer, M
Kratschmer, I
Liko, D
Matsushita, T
Mikulec, I
Rabady, D
Rad, N
Rahbaran, B
Rohringer, H
Schieck, J
Strauss, J
Treberer-Treberspurg, W
Waltenberger, W
Wulz, CE
Mossolov, V
Shumeiko, N
Gonzalez, JS
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Cornelis, T
De Wolf, EA
Janssen, X
Knutsson, A
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Van De Klundert, M
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Blekman, F
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CA CMS Collaboration
TI Measurement of the integrated and differential t(t)over-bar production
cross sections for high-p(T) top quarks in pp collisions at root s=8 TeV
SO PHYSICAL REVIEW D
LA English
DT Article
ID PARTON DISTRIBUTIONS; LHC
AB The cross section for pair production of top quarks (t (t) over bar) with high transverse momenta is measured in pp collisions, collected with the CMS detector at the LHC with root s = 8 TeV in data corresponding to an integrated luminosity of 19.7 fb(-1). The measurement is performed using lepton + jets events, where one top quark decays semileptonically, while the second top quark decays to a hadronic final state. The hadronic decay is reconstructed as a single, large-radius jet, and identified as a top quark candidate using jet substructure techniques. The integrated cross section and the differential cross sections as a function of top quark pT and rapidity are measured at particle level within a fiducial region related to the detector-level requirements and at parton level. The particle-level integrated cross section is found to be sigma t (t) over bar = 0.499 + 0.035 (stat + syst) +/- 0.095 (theo) + 0.013 (lumi) pb for top quark p(T) > 400 GeV. The parton-level measurement is sigma t (t) over bar = 1.44 +/- 0.10 (stat + syst) + 0.29 (theo) + 0.04 (lumi) pb. The integrated and differential cross section results are compared to predictions from several event generators.
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[Adam, W.; Asilar, E.; Bergauer, T.; Brandstetter, J.; Brondolin, E.; Dragicevic, M.; Eroe, J.; Flechl, M.; Friedl, M.; Fruhwirth, R.; Ghete, V. M.; Hartl, C.; Hoermann, N.; Hrubec, J.; Jeitler, M.; Koenig, A.; Krammer, M.; Kraetschmer, I.; Liko, D.; Matsushita, T.; Mikulec, I.; Rabady, D.; Rad, N.; Rahbaran, B.; Rohringer, H.; Schieck, J.; Strauss, J.; Treberer-Treberspurg, W.; Waltenberger, W.; Wulz, C. -E.] OeAW, Inst Hochenergiephys, Vienna, Austria.
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[Abu Zeid, S.; Blekman, F.; D'Hondt, J.; Daci, N.; De Bruyn, I.; Deroover, K.; Heracleous, N.; Keaveney, J.; Lowette, S.; Moortgat, S.; Moreels, L.; Olbrechts, A.; Python, Q.; Strom, D.; Tavernier, S.; Van Doninck, W.; Van Mulders, P.; Van Parijs, I.] Vrije Univ Brussel, Brussels, Belgium.
[Brun, H.; Caillol, C.; Clerbaux, B.; De Lentdecker, G.; Fasanella, G.; Favart, L.; Goldouzian, R.; Grebenyuk, A.; Karapostoli, G.; Lenzi, T.; Leonard, A.; Maerschalk, T.; Marinov, A.; Randle-Conde, A.; Seva, T.; Velde, C. Vander; Vanlaer, P.; Yonamine, R.; Zenoni, F.; Zhang, F.] Univ Libre Bruxelles, Brussels, Belgium.
[Benucci, L.; Cimmino, A.; Crucy, S.; Dobur, D.; Fagot, A.; Garcia, G.; Gul, M.; Mccartin, J.; Rios, A. A. Ocampo; Poyraz, D.; Ryckbosch, D.; Salva, S.; Schofbeck, R.; Sigamani, M.; Tytgat, M.; Van Driessche, W.; Yazgan, E.; Zaganidis, N.] Univ Ghent, Ghent, Belgium.
[Beluffi, C.; Bondu, O.; Brochet, S.; Bruno, G.; Caudron, A.; Ceard, L.; De Visscher, S.; Delaere, C.; Delcourt, M.; Favart, D.; Forthomme, L.; Giammanco, A.; Jafari, A.; Jez, P.; Komm, M.; Lemaitre, V.; Mertens, A.; Musich, M.; Nuttens, C.; Piotrzkowski, K.; Quertenmont, L.; Selvaggi, M.; Marono, M. Vidal; Beliy, N.] Catholic Univ Louvain, Louvain La Neuve, Belgium.
[Hammad, G. H.] Univ Mons, Mons, Belgium.
[Alda, W. L., Jr.; Alves, F. L.; Alves, G. A.; Brito, L.; Martins, M. Correa, Jr.; Hamer, M.; Hensel, C.; Moraes, A.; Pol, M. E.; Teles, P. Rebello] Ctr Brasileiro Pesquisas Fis, Rio De Janeiro, Brazil.
[Das Chagas, E. Belchior Batista; Carvalho, W.; Chinellato, J.; Custodio, A.; Da Costa, E. M.; Damiao, D. De Jesus; Martins, C. De Oliveira; De Souza, S. Fonseca; Guativa, L. M. Huertas; Malbouisson, H.; Figueiredo, D. Matos; Herrera, C. Mora; Mundim, L.; Nogima, H.; Da Silva, W. L. Prado; Santoro, A.; Sznajder, A.; Manganote, E. J. Tonelli; Pereira, A. Vilela] Univ Estado Rio de Janeiro, Rio De Janeiro, Brazil.
[Ahuja, S.; Dogra, S.; Tomei, T. R. Fernandez Perez; Moon, C. S.; Novaes, S. F.; Padula, Sandra S.; Vargas, J. C. Ruiz] Univ Estadual Paulista, Sao Paulo, Brazil.
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[Aleksandrov, A.; Hadjiiska, R.; Iaydjiev, P.; Rodozov, M.; Stoykova, S.; Sultanov, G.; Vutova, M.] Inst Nucl Energy Res, Sofia, Bulgaria.
[Dimitrov, A.; Glushkov, I.; Litov, L.; Pavlov, B.; Petkov, P.] Univ Sofia, Sofia, Bulgaria.
[Fang, W.] Beihang Univ, Beijing, Peoples R China.
[Ahmad, M.; Bian, J. G.; Chen, G. M.; Chen, H. S.; Chen, M.; Cheng, T.; Du, R.; Jiang, C. H.; Leggat, D.; Plestina, R.; Romeo, F.; Shaheen, S. M.; Spiezia, A.; Tao, J.; Wang, C.; Wang, Z.; Zhang, H.] Inst High Energy Phys, Beijing, Peoples R China.
[Asawatangtrakuldee, C.; Ban, Y.; Li, Q.; Liu, S.; Mao, Y.; Qian, S. J.; Wang, D.; Xu, Z.] Peking Univ, State Key Lab Nucl Phys & Technol, Beijing, Peoples R China.
[Avila, C.; Cabrera, A.; Sierra, L. F. Chaparro; Florez, C.; Gomez, J. P.; Moreno, B. Gomez; Sanabria, J. C.] Univ Los Andes, Bogota, Colombia.
[Godinovic, N.; Lelas, D.; Puljak, I.; Cipriano, P. M. Ribeiro] Univ Split, Fac Elect Engn Mech Engn & Naval Architecture, Split, Croatia.
[Antunovic, Z.; Kovac, M.] Univ Split, Fac Sci, Split, Croatia.
[Brigljevic, V.; Ferencek, D.; Kadija, K.; Luetic, J.; Micanovic, S.; Sudic, L.] Inst Rudjer Boskov, Zagreb, Croatia.
[Attikis, A.; Mavromanolakis, G.; Mousa, J.; Nicolaou, C.; Ptochos, F.; Razis, P. A.; Rykaczewski, H.] Univ Cyprus, Nicosia, Cyprus.
[Finger, M.; Finger, M., Jr.] Charles Univ Prague, Prague, Czech Republic.
[Jarrin, E. Carrera] Univ San Francisco Quito, Quito, Ecuador.
[Assran, Y.; Kamel, A. Ellithi; Mahrous, A.; Radi, A.] Acad Sci Res & Technol Arab Republ Egypt, Egyptian Network High Energy Phys, Cairo, Egypt.
[Calpas, B.; Kadastik, M.; Murumaa, M.; Perrini, L.; Raidal, M.; Tiko, A.; Veelken, C.] NICPB, Tallinn, Estonia.
[Eerola, P.; Pekkanen, J.; Voutilainen, M.] Univ Helsinki, Dept Phys, Helsinki, Finland.
[Harkonen, J.; Karimaki, V.; Kinnunen, R.; Lampen, T.; Lassila-Perini, K.; Lehti, S.; Linden, T.; Luukka, P.; Peltola, T.; Tuominiemi, J.; Tuovinen, E.; Wendland, L.] Helsinki Inst Phys, Helsinki, Finland.
[Talvitie, J.; Tuuva, T.] Lappeenranta Univ Technol, Lappeenranta, Finland.
[Besancon, M.; Couderc, F.; Dejardin, M.; Denegri, D.; Fabbro, B.; Faure, J. L.; Favaro, C.; Ferri, F.; Ganjour, S.; Givernaud, A.; Gras, P.; de Monchenault, G. Hamel; Jarry, P.; Locci, E.; Machet, M.; Malcles, J.; Rander, J.; Rosowsky, A.; Titov, M.; Zghiche, A.] CEA Saclay, DSM IRFU, Gif Sur Yvette, France.
[Abdulsalam, A.; Antropov, I.; Baffioni, S.; Beaudette, F.; Busson, P.; Cadamuro, L.; Chapon, E.; Charlot, C.; Davignon, O.; Dobrzynski, L.; de Cassagnac, R. Granier; Jo, M.; Lisniak, S.; Mine, P.; Naranjo, I. N.; Nguyen, M.; Ochando, C.; Ortona, G.; Paganini, P.; Pigard, P.; Regnard, S.; Salerno, R.; Sirois, Y.; Strebler, T.; Yilmaz, Y.; Zabi, A.] Ecole Polytech, Lab Leprince Ringuet, CNRS, IN2P3, Palaiseau, France.
[Agram, J. -L.; Andrea, J.; Aubin, A.; Bloch, D.; Brom, J. -M.; Buttignol, M.; Chabert, E. C.; Chanon, N.; Collard, C.; Conte, E.; Coubez, X.; Fontaine, J. -C.; Gele, D.; Goerlach, U.; Goetzmann, C.; Le Bihan, A. -C.; Merlin, J. A.; Skovpen, K.; Van Hove, P.] Univ Haute Alsace Mulhouse, Univ Strasbourg, Inst Pluridisciplinaire Hubert Curien, CNRS,IN2P3, Strasbourg, France.
[Gadrat, S.] Inst Natl Phys Nucl & Phys Particules, Ctr Calcul, CNRS, IN2P3, Villeurbanne, France.
[Beauceron, S.; Bernet, C.; Boudoul, G.; Bouvier, E.; Montoya, C. A. Carrillo; Chierici, R.; Contardo, D.; Courbon, B.; Depasse, P.; El Mamouni, H.; Fan, J.; Fay, J.; Gascon, S.; Gouzevitch, M.; Ille, B.; Lagarde, F.; Laktineh, I. B.; Lethuillier, M.; Mirabito, L.; Pequegnot, A. L.; Perries, S.; Popov, A.; Alvarez, J. D. Ruiz; Sabes, D.; Sordini, V.; Donckt, M. Vander; Verdier, P.; Viret, S.] Univ Claude Bernard Lyon 1, Univ Lyon, CNRS, IN2P3,Inst Phys Nucl Lyon, Villeurbanne, France.
[Toriashvili, T.] Georgian Tech Univ, Tbilisi, Rep of Georgia.
[Tsamalaidze, Z.] Tbilisi State Univ, Tbilisi, Rep of Georgia.
[Autermann, C.; Beranek, S.; Feld, L.; Heister, A.; Kiesel, M. K.; Klein, K.; Lipinski, M.; Ostapchuk, A.; Preuten, M.; Raupach, F.; Schael, S.; Schomakers, C.; Schulte, J. F.; Schulz, J.; Verlage, T.; Weber, H.; Zhukov, V.] Rhein Westfal TH Aachen, Inst Phys 1, Aachen, Germany.
[Ata, M.; Brodski, M.; Dietz-Laursonn, E.; Duchardt, D.; Endres, M.; Erdmann, M.; Erdweg, S.; Esch, T.; Fischer, R.; Gueth, A.; Hebbeker, T.; Heidemann, C.; Hoepfner, K.; Knutzen, S.; Merschmeyer, M.; Meyer, A.; Millet, P.; Mukherjee, S.; Olschewski, M.; Padeken, K.; Papacz, P.; Pook, T.; Radziej, M.; Reithler, H.; Rieger, M.; Scheuch, F.; Sonnenschein, L.; Teyssier, D.; Thueer, S.] Rhein Westfal TH Aachen, Phys Inst A3, Aachen, Germany.
[Cherepanov, V.; Erdogan, Y.; Fluegge, G.; Geenen, H.; Geisler, M.; Hoehle, F.; Kargoll, B.; Kress, T.; Kuensken, A.; Lingemann, J.; Nehrkorn, A.; Nowack, A.; Nugent, I. M.; Pistone, C.; Pooth, O.; Stahl, A.] Rhein Westfal TH Aachen, Phys Inst B3, Aachen, Germany.
[Martin, M. Aldaya; Asin, I.; Beernaert, K.; Behnke, O.; Behrens, U.; Borras, K.; Campbell, A.; Connor, P.; Contreras-Campana, C.; Costanza, F.; Pardos, C. Diez; Dolinska, G.; Dooling, S.; Eckerlin, G.; Eckstein, D.; Eichhorn, T.; Gallo, E.; Garcia, J. Garay; Geiser, A.; Gizhko, A.; Luyando, J. M. Grados; Gunnellini, P.; Harb, A.; Hauk, J.; Hempel, M.; Jung, H.; Kalogeropoulos, A.; Karacheban, O.; Kasemann, M.; Kieseler, J.; Kleinwort, C.; Korol, I.; Lange, W.; Lelek, A.; Leonard, J.; Lipka, K.; Lobanov, A.; Lohmann, W.; Mankel, R.; Melzer-Pellmann, I. -A.; Meyer, A. B.; Mittag, G.; Mnich, J.; Mussgiller, A.; Ntomari, E.; Pitzl, D.; Placakyte, R.; Raspereza, A.; Roland, B.; Sahin, M. O.; Saxena, P.; Schoerner-Sadenius, T.; Seitz, C.; Spannagel, S.; Stefaniuk, N.; Trippkewitz, K. D.; Van Onsem, G. P.; Walsh, R.; Wissing, C.] DESY, Hamburg, Germany.
[Abdulsalam, A.; Blobel, V.; Vignali, M. Centis; Draeger, A. R.; Dreyer, T.; Erfle, J.; Garutti, E.; Goebel, K.; Gonzalez, D.; Gorner, M.; Haller, J.; Hoffmann, M.; Hoing, R. S.; Junkes, A.; Klanner, R.; Kogler, R.; Kovalchuk, N.; Lapsien, T.; Lenz, T.; Marchesini, I.; Marconi, D.; Meyer, M.; Niedziela, M.; Nowatschin, D.; Ott, J.; Pantaleo, F.; Peiffer, T.; Perieanu, A.; Pietsch, N.; Poehlsen, J.; Sander, C.; Scharf, C.; Schleper, P.; Schlieckau, E.; Schmidt, A.; Schumann, S.; Schwandt, J.; Stadie, H.; Steinbruck, G.; Stober, F. M.; Tholen, H.; Troendle, D.; Usai, E.; Vanelderen, L.; Vanhoefer, A.; Vormwald, B.] Univ Hamburg, Hamburg, Germany.
[Abdulsalam, A.; Barth, C.; Baus, C.; Berger, J.; Boser, C.; Butz, E.; Chwalek, T.; Colombo, F.; De Boer, W.; Descroix, A.; Dierlamm, A.; Fink, S.; Frensch, F.; Friese, R.; Giffels, M.; Gilbert, A.; Haitz, D.; Hartmann, F.; Heindl, S. M.; Husemann, U.; Katkov, I.; Kornmayer, A.; Pardo, P. Lobelle; Maier, B.; Mildner, H.; Mozer, M. U.; Muller, T.; Muller, Th.; Plagge, M.; Quast, G.; Rabbertz, K.; Rocker, S.; Roscher, F.; Schroder, M.; Sieber, G.; Simonis, H. J.; Ulrich, R.; Wagner-Kuhr, J.; Wayand, S.; Weber, M.; Weiler, T.; Williamson, S.; Wohrmann, C.; Wolf, R.; Ackert, A.] Inst Expt Kernphys, Karlsruhe, Germany.
[Anagnostou, G.; Daskalakis, G.; Geralis, T.; Giakoumopoulou, V. A.; Kyriakis, A.; Loukas, D.; Psallidas, A.; Topsis-Giotis, I.] NCSR Demokritos, INPP, Aghia Paraskevi, Greece.
[Agapitos, A.; Kesisoglou, S.; Panagiotou, A.; Saoulidou, N.; Tziaferi, E.] Univ Athens, Athens, Greece.
[Evangelou, I.; Flouris, G.; Foudas, C.; Kokkas, P.; Loukas, N.; Manthos, N.; Papadopoulos, I.; Paradas, E.; Strologas, J.] Univ Ioannina, Ioannina, Greece.
[Filipovic, N.] Eotvos Lorand Univ, MTA ELTE Lendlet CMS Particle & Nucl Phys Grp, Budapest, Hungary.
[Bencze, G.; Hajdu, C.; Hidas, P.; Horvath, D.; Sikler, F.; Veszpremi, V.; Vesztergombi, G.; Zsigmond, A. J.] Wigner Res Ctr Phys, Budapest, Hungary.
[Beni, N.; Czellar, S.; Karancsi, J.; Molnar, J.; Szillasi, Z.] Inst Nucl Res ATOMKI, Debrecen, Hungary.
[Bartok, M.; Makovec, A.; Raics, P.; Trocsanyi, Z. L.; Ujvari, B.] Univ Debrecen, Debrecen, Hungary.
[Choudhury, S.; Mal, P.; Mandal, K.; Nayak, A.; Sahoo, D. K.; Sahoo, N.; Swain, S. K.] Natl Inst Sci Educ & Res, Bhubaneswar, Orissa, India.
[Bansal, S.; Beri, S. B.; Bhatnagar, V.; Chawla, R.; Gupta, R.; Bhawandeep, U.; Kalsi, A. K.; Kaur, A.; Kaur, M.; Kumar, R.; Mehta, A.; Mittal, M.; Singh, J. B.; Walia, G.] Panjab Univ, Chandigarh, India.
[Kumar, Ashok; Bhardwaj, A.; Choudhary, B. C.; Garg, R. B.; Keshri, S.; Kumar, A.; Malhotra, S.; Naimuddin, M.; Nishu, N.; Ranjan, K.; Sharma, R.; Sharma, V.] Univ Delhi, Delhi, India.
[Bhattacharya, R.; Bhattacharya, S.; Chatterjee, K.; Dey, S.; Dutta, S.; Ghosh, S.; Majumdar, N.; Modak, A.; Mondal, K.; Mukhopadhyay, S.; Nandan, S.; Purohit, A.; Roy, A.; Roy, D.; Chowdhury, S. Roy; Sarkar, S.; Sharan, M.] Saha Inst Nucl Phys, Kolkata, India.
[Chudasama, R.; Dutta, D.; Jha, V.; Kumar, V.; Mohanty, A. K.; Pant, L. M.; Shukla, P.; Topkar, A.] Bhabha Atom Res Ctr, Mumbai, Maharashtra, India.
[Aziz, T.; Banerjee, S.; Bhowmik, S.; Chatterjee, R. M.; Dewanjee, R. K.; Dugad, S.; Ganguly, S.; Ghosh, S.; Guchait, M.; Gurtu, A.; Jain, Sa.; Kole, G.; Kumar, S.; Mahakud, B.; Maity, M.; Majumder, G.; Mazumdar, K.; Mitra, S.; Mohanty, G. B.; Parida, B.; Sarkar, T.; Sur, N.; Sutar, B.; Wickramage, N.] Tata Inst Fundamental Res, Mumbai, Maharashtra, India.
[Chauhan, S.; Dube, S.; Kapoor, A.; Kothekar, K.; Rane, A.; Sharma, S.] IISER, Pune, Maharashtra, India.
[Bakhshiansohi, H.; Behnamian, H.; Etesami, S. M.; Fahim, A.; Khakzad, M.; Najafabadi, M. Mohammadi; Naseri, M.; Mehdiabadi, S. Paktinat; Hosseinabadi, F. Rezaei; Safarzadeh, B.; Zeinali, M.] Inst Res Fundamental Sci IPM, Tehran, Iran.
[Felcini, M.; Grunewald, M.] Univ Coll Dublin, Dublin, Ireland.
[Abbrescia, M.; Calabria, C.; Caputo, C.; Colaleo, A.; Creanza, D.; Cristella, L.; De Filippis, N.; De Palma, M.; Fiore, L.; Iaselli, G.; Maggi, G.; Maggi, M.; Miniello, G.; My, S.; Nuzzo, S.; Pompili, A.; Pugliese, G.; Radogna, R.; Ranieri, A.; Selvaggi, G.; Silvestris, L.; Venditti, R.] Ist Nazl Fis Nucl, Sez Bari, Bari, Italy.
[Abbrescia, M.; Calabria, C.; Caputo, C.; Cristella, L.; De Palma, M.; Miniello, G.; My, S.; Nuzzo, S.; Pompili, A.; Radogna, R.; Selvaggi, G.; Venditti, R.] Univ Bari, Bari, Italy.
[Creanza, D.; De Filippis, N.; Iaselli, G.; Maggi, G.; Pugliese, G.] Politecn Bari, Bari, Italy.
[Abbiendi, G.; Battilana, C.; Bonacorsi, D.; Braibant-Giacomelli, S.; Brigliadori, L.; Campanini, R.; Capiluppi, P.; Castro, A.; Cavallo, F. R.; Chhibra, S. S.; Codispoti, G.; Cuffiani, M.; Dallavalle, G. M.; Fabbri, F.; Fanfani, A.; Fasanella, D.; Giacomelli, P.; Grandi, C.; Guiducci, L.; Marcellini, S.; Masetti, G.; Montanari, A.; Navarria, F. L.; Perrotta, A.; Rossi, A. M.; Rovelli, T.; Siroli, G. P.; Tosi, N.] Ist Nazl Fis Nucl, Sez Bologna, Bologna, Italy.
[Bonacorsi, D.; Braibant-Giacomelli, S.; Brigliadori, L.; Campanini, R.; Capiluppi, P.; Castro, A.; Chhibra, S. S.; Codispoti, G.; Cuffiani, M.; Fanfani, A.; Fasanella, D.; Guiducci, L.; Navarria, F. L.; Rossi, A. M.; Rovelli, T.; Siroli, G. P.; Tosi, N.] Univ Bologna, Bologna, Italy.
[Chiorboli, M.; Costa, S.; Di Mattia, A.; Giordano, F.; Potenza, R.; Tricomi, A.; Tuve, C.] Ist Nazl Fis Nucl, Sez Catania, Catania, Italy.
[Cappello, G.; Chiorboli, M.; Costa, S.; Giordano, F.; Potenza, R.; Tricomi, A.; Tuve, C.] Univ Catania, Catania, Italy.
[Barbagli, G.; Ciulli, V.; Civinini, C.; D'Alessandro, R.; Focardi, E.; Gori, V.; Lenzi, P.; Meschini, M.; Paoletti, S.; Sguazzoni, G.; Viliani, L.] Ist Nazl Fis Nucl, Sez Firenze, Florence, Italy.
[Ciulli, V.; D'Alessandro, R.; Focardi, E.; Gori, V.; Lenzi, P.; Viliani, L.] Univ Florence, Florence, Italy.
[Benussi, L.; Bianco, S.; Fabbri, F.; Piccolo, D.; Primavera, F.] Ist Nazl Fis Nucl, Lab Nazl Frascati, Frascati, Italy.
[Calvelli, V.; Ferro, F.; Lo Vetere, M.; Monge, M. R.; Robutti, E.; Tosi, S.] Ist Nazl Fis Nucl, Sez Genova, Genoa, Italy.
[Calvelli, V.; Lo Vetere, M.; Monge, M. R.; Tosi, S.] Univ Genoa, Genoa, Italy.
[Brianza, L.; Dinardo, M. E.; Fiorendi, S.; Gennai, S.; Ghezzi, A.; Govoni, P.; Malvezzi, S.; Manzoni, R. A.; Marzocchi, B.; Menasce, D.; Moroni, L.; Paganoni, M.; Pedrini, D.; Pigazzini, S.; Ragazzi, S.; Redaelli, N.; de Fatis, T. Tabarelli] Ist Nazl Fis Nucl, Sez Milano Bicocca, Milan, Italy.
[Dinardo, M. E.; Fiorendi, S.; Ghezzi, A.; Govoni, P.; Manzoni, R. A.; Marzocchi, B.; Paganoni, M.; Ragazzi, S.; de Fatis, T. Tabarelli] Univ Milano Bicocca, Milan, Italy.
[Buontempo, S.; Cavallo, N.; Di Guida, S.; Esposito, M.; Fabozzi, F.; Iorio, A. O. M.; Lanza, G.; Lista, L.; Meola, S.; Merola, M.; Paolucci, P.; Sciacca, C.; Thyssen, F.] Ist Nazl Fis Nucl, Sez Napoli, Rome, Italy.
[Esposito, M.; Iorio, A. O. M.; Sciacca, C.] Univ Naples Federico II, Rome, Italy.
[Cavallo, N.; Fabozzi, F.] Univ Basilicata, Rome, Italy.
[Di Guida, S.; Meola, S.] Univ G Marconi, Rome, Italy.
[Azzi, P.; Bacchetta, N.; Bellato, M.; Benato, L.; Bisello, D.; Boletti, A.; Carlin, R.; Checchia, P.; Dall'Osso, M.; Manzano, P. De Castro; Dorigo, T.; Dosselli, U.; Fantinel, S.; Gasparini, F.; Gasparini, U.; Gozzelino, A.; Lacaprara, S.; Margoni, M.; Meneguzzo, A. T.; Pazzini, J.; Pozzobon, N.; Ronchese, P.; Simonetto, F.; Torassa, E.; Tosi, M.; Ventura, S.; Zanetti, M.; Zotto, P.; Zucchetta, A.; Zumerle, G.] Ist Nazl Fis Nucl, Sez Padova, Trento, Italy.
[Benato, L.; Bisello, D.; Boletti, A.; Carlin, R.; Dall'Osso, M.; Gasparini, F.; Gasparini, U.; Margoni, M.; Meneguzzo, A. T.; Pazzini, J.; Pozzobon, N.; Ronchese, P.; Simonetto, F.; Tosi, M.; Zotto, P.; Zucchetta, A.; Zumerle, G.] Univ Padua, Trento, Italy.
Univ Trento, Trento, Italy.
[Braghieri, A.; Magnani, A.; Montagna, P.; Ratti, S. P.; Re, V.; Riccardi, C.; Salvini, P.; Vai, I.; Vitulo, P.] Ist Nazl Fis Nucl, Sez Pavia, Pavia, Italy.
[Magnani, A.; Montagna, P.; Ratti, S. P.; Riccardi, C.; Vai, I.; Vitulo, P.] Univ Pavia, Pavia, Italy.
[Solestizi, L. Alunni; Bilei, G. M.; Ciangottini, D.; Fano, L.; Lariccia, P.; Leonardi, R.; Mantovani, G.; Menichelli, M.; Saha, A.; Santocchia, A.] Ist Nazl Fis Nucl, Sez Perugia, Perugia, Italy.
[Solestizi, L. Alunni; Ciangottini, D.; Fano, L.; Lariccia, P.; Leonardi, R.; Mantovani, G.; Santocchia, A.] Univ Perugia, Perugia, Italy.
[Androsov, K.; Azzurri, P.; Bagliesi, G.; Bernardini, J.; Boccali, T.; Castaldi, R.; Ciocci, M. A.; Dell'Orso, R.; Donato, S.; Fedi, G.; Giassi, A.; Grippo, M. T.; Ligabue, F.; Lomtadze, T.; Martini, L.; Messineo, A.; Palla, F.; Rizzi, A.; Savoy-Navarro, A.; Spagnolo, P.; Tenchini, R.; Tonelli, G.; Venturi, A.; Verdini, P. G.] Ist Nazl Fis Nucl, Sez Pisa, Pisa, Italy.
[Martini, L.; Messineo, A.; Rizzi, A.; Tonelli, G.] Univ Pisa, Pisa, Italy.
[Ligabue, F.] Scuola Normale Super Pisa, Pisa, Italy.
[Barone, L.; Cavallari, F.; D'imperio, G.; Del Re, D.; Diemoz, M.; Gelli, S.; Jorda, C.; Longo, E.; Margaroli, F.; Meridiani, P.; Organtini, G.; Paramatti, R.; Preiato, F.; Rahatlou, S.; Rovelli, C.; Santanastasio, F.] Ist Nazl Fis Nucl, Sez Roma, Rome, Italy.
[Barone, L.; D'imperio, G.; Del Re, D.; Gelli, S.; Longo, E.; Margaroli, F.; Organtini, G.; Preiato, F.; Rahatlou, S.; Santanastasio, F.] Univ Rome, Rome, Italy.
[Amapane, N.; Arcidiacono, R.; Argiro, S.; Arneodo, M.; Bartosik, N.; Bellan, R.; Biino, C.; Cartiglia, N.; Costa, M.; Covarelli, R.; Degano, A.; Demaria, N.; Finco, L.; Kiani, B.; Mariotti, C.; Maselli, S.; Migliore, E.; Monaco, V.; Monteil, E.; Obertino, M. M.; Pacher, L.; Pastrone, N.; Pelliccioni, M.; Angioni, G. L. Pinna; Ravera, F.; Romero, A.; Ruspa, M.; Sacchi, R.; Sola, V.; Solano, A.; Staiano, A.] Ist Nazl Fis Nucl, Sez Torino, Novara, Italy.
[Amapane, N.; Argiro, S.; Bellan, R.; Costa, M.; Covarelli, R.; Degano, A.; Finco, L.; Kiani, B.; Migliore, E.; Monaco, V.; Monteil, E.; Obertino, M. M.; Pacher, L.; Angioni, G. L. Pinna; Ravera, F.; Romero, A.; Sacchi, R.; Solano, A.] Univ Turin, Novara, Italy.
[Arcidiacono, R.; Arneodo, M.; Ruspa, M.] Univ Piemonte Orientale, Novara, Italy.
[Belforte, S.; Candelise, V.; Casarsa, M.; Cossutti, F.; Della Ricca, G.; La Licata, C.; Schizzi, A.; Zanetti, A.] Ist Nazl Fis Nucl, Sez Trieste, Trieste, Italy.
[Candelise, V.; Della Ricca, G.; La Licata, C.; Schizzi, A.] Univ Trieste, Trieste, Italy.
[Nam, S. K.] Kangwon Natl Univ, Chunchon, South Korea.
[Kim, D. H.; Kim, G. N.; Kim, M. S.; Kong, D. J.; Lee, S.; Lee, S. W.; Oh, Y. D.; Sakharov, A.; Son, D. C.] Kyungpook Natl Univ, Daegu, South Korea.
[Cifuentes, J. A. Brochero; Kim, H.; Kim, T. J.] Chonbuk Natl Univ, Jeonju, South Korea.
[Song, S.] Chonnam Natl Univ, Inst Universe & Elementary Particles, Kwangju, South Korea.
[Cho, S.; Choi, S.; Go, Y.; Gyun, D.; Hong, B.; Kim, Y.; Lee, B.; Lee, K.; Lee, K. S.; Lee, S.; Lim, J.; Park, S. K.; Roh, Y.] Korea Univ, Seoul, South Korea.
[Yoo, H. D.] Seoul Natl Univ, Seoul, South Korea.
[Choi, M.; Kim, J. H.; Lee, J. S. H.; Park, I. C.; Ryu, G.; Ryu, M. S.] Univ Seoul, Seoul, South Korea.
[Choi, Y.; Goh, J.; Kim, D.; Kwon, E.; Lee, J.; Yu, I.] Sungkyunkwan Univ, Suwon, South Korea.
[Dudenas, V.; Juodagalvis, A.; Vaitkus, J.] Vilnius Univ, Vilnius, Lithuania.
[Ahmed, I.; Ibrahim, Z. A.; Komaragiri, J. R.; Ali, M. A. B. Md; Idris, F. Mohamad; Abdullah, W. A. T. Wan; Yusli, M. N.; Zolkapli, Z.] Univ Malaya, Natl Ctr Particle Phys, Kuala Lumpur, Malaysia.
[Linares, E. Casimiro; Castilla-Valdez, H.; De La Cruz-Burelo, E.; Heredia-De La Cruz, I.; Hernandez-Almada, A.; Lopez-Fernandez, R.; Guisao, J. Mejia; Sanchez-Hernandez, A.] IPN, Ctr Invest & Estudios Avanzados, Mexico City, DF, Mexico.
[Moreno, S. Carrillo; Valencia, F. Vazquez] Univ Iberoamer, Mexico City, DF, Mexico.
[Pedraza, I.; Ibarguen, H. A. Salazar; Estrada, C. Uribe] Benemerita Univ Autonoma Puebla, Puebla, Mexico.
[Krofcheck, D.] Univ Auckland, Auckland, New Zealand.
[Butler, P. H.] Univ Canterbury, Christchurch, New Zealand.
[Bialkowska, H.; Bluj, M.; Boimska, B.; Frueboes, T.; Gorski, M.; Kazana, M.; Nawrocki, K.; Romanowska-Rybinska, K.; Szleper, M.; Traczyk, P.; Zalewski, P.] Natl Ctr Nucl Res, Otwock, Poland.
[Brona, G.; Bunkowski, K.; Byszuk, A.; Doroba, K.; Kalinowski, A.; Konecki, M.; Krolikowski, J.; Misiura, M.; Olszewski, M.; Walczak, M.] Univ Warsaw, Inst Expt Phys, Fac Phys, Warsaw, Poland.
[Bargassa, P.; Da Cruz E Silva, C. Beirao; Di Francesco, A.; Faccioli, P.; Ferreira Parracho, P. G.; Gallinaro, M.; Hollar, J.; Leonardo, N.; Iglesias, L. Lloret; Nemallapudi, M. V.; Nguyen, F.; Antunes, J. Rodrigues; Seixas, J.; Toldaiev, O.; Vadruccio, D.; Varela, J.; Vischia, P.] Lab Instrumentacao & Fis Expt Particulas, Lisbon, Portugal.
[Bunin, P.; Golutvin, I.; Kamenev, A.; Karjavin, V.; Korenkov, V.; Lanev, A.; Malakhov, A.; Matveev, V.; Mitsyn, V. V.; Moisenz, P.; Palichik, V.; Perelygin, V.; Shmatov, S.; Shulha, S.; Skatchkov, N.; Smirnov, V.; Tikhonenko, E.; Voytishin, N.; Zarubin, A.] Joint Inst Nucl Res, Dubna, Russia.
[Golovtsov, V.; Ivanov, Y.; Kim, V.; Kuznetsova, E.; Levchenko, P.; Murzin, V.; Oreshkin, V.; Smirnov, I.; Sulimov, V.; Uvarov, L.; Vavilov, S.; Vorobyev, A.] Petersburg Nucl Phys Inst, St Petersburg, Russia.
[Andreev, Yu.; Dermenev, A.; Gninenko, S.; Golubev, N.; Karneyeu, A.; Kirsanov, M.; Krasnikov, N.; Pashenkov, A.; Tlisov, D.; Toropin, A.] Inst Nucl Res, Moscow, Russia.
[Epshteyn, V.; Gavrilov, V.; Lychkovskaya, N.; Popov, V.; Pozdnyakov, I.; Safronov, G.; Spiridonov, A.; Toms, M.; Vlasov, E.; Zhokin, A.] Inst Theoret & Expt Phys, Moscow, Russia.
[Chadeeva, M.; Chistov, R.; Danilov, M.; Rusinov, V.; Tarkovskii, E.] Natl Res Nucl Univ, Moscow Engn Phys Inst MEPhI, Moscow, Russia.
[Andreev, V.; Azarkin, M.; Dremin, I.; Kirakosyan, M.; Leonidov, A.; Mesyats, G.; Rusakov, S. V.] PN Lebedev Phys Inst, Moscow, Russia.
[Baskakov, A.; Belyaev, A.; Boos, E.; Bunichev, V.; Dubinin, M.; Dudko, L.; Ershov, A.; Klyukhin, V.; Korneeva, N.; Lokhtin, I.; Miagkov, I.; Obraztsov, S.; Perfilov, M.; Petrushanko, S.; Savrin, V.] Lomonosov Moscow State Univ, Skobeltsyn Inst Nucl Phys, Moscow, Russia.
[Azhgirey, I.; Bayshev, I.; Bitioukov, S.; Kachanov, V.; Kalinin, A.; Konstantinov, D.; Krychkine, V.; Petrov, V.; Ryutin, R.; Sobol, A.; Tourtchanovitch, L.; Troshin, S.; Tyurin, N.; Uzunian, A.; Volkov, A.] State Res Ctr Russian Federat, Inst High Energy Phys, Protvino, Russia.
[Adzic, P.; Cirkovic, P.; Devetak, D.; Milosevic, J.; Rekovic, V.] Univ Belgrade, Fac Phys, Belgrade, Serbia.
[Adzic, P.; Cirkovic, P.; Devetak, D.; Milosevic, J.; Rekovic, V.] Vinca Inst Nucl Sci, Belgrade, Serbia.
[Alcaraz Maestre, J.; Calvo, E.; Cerrada, M.; Chamizo Llatas, M.; Colino, N.; De La Cruz, B.; Delgado Peris, A.; Escalante Del Valle, A.; Fernandez Bedoya, C.; Fernandez Ramos, J. P.; Flix, J.; Fouz, M. C.; Garcia-Abia, P.; Gonzalez Lopez, O.; Goy Lopez, S.; Hernandez, J. M.; Josa, M. I.; Navarro De Martino, E.; Perez-Calero Yzquierdo, A.; Puerta Pelayo, J.; Quintario Olmeda, A.; Redondo, I.; Romero, L.; Soares, M. S.] CIEMAT, Madrid, Spain.
[de Troconiz, J. F.; Missiroli, M.; Moran, D.] Univ Autonoma Madrid, Madrid, Spain.
[Cuevas, J.; Fernandez Menendez, J.; Folgueras, S.; Gonzalez Caballero, I.; Palencia Cortezon, E.; Vizan Garcia, J. M.] Univ Oviedo, Oviedo, Spain.
[Cabrillo, I. J.; Calderon, A.; Castineiras De Saa, J. R.; Curras, E.; Fernandez, M.; Garcia-Ferrero, J.; Gomez, G.; Lopez Virto, A.; Marco, J.; Marco, R.; Martinez Rivero, C.; Matorras, F.; Piedra Gomez, J.; Rodrigo, T.; Rodriguez-Marrero, A. Y.; Ruiz-Jimeno, A.; Scodellaro, L.; Trevisani, N.; Vila, I.; Vilar Cortabitarte, R.] Univ Cantabria, CSIC, Inst Fis Cantabria IFCA, Santander, Spain.
[Abbaneo, D.; Auffray, E.; Auzinger, G.; Bachtis, M.; Baillon, P.; Ball, A. H.; Barney, D.; Benaglia, A.; Benhabib, L.; Berruti, G. M.; Bloch, P.; Bocci, A.; Bonato, A.; Botta, C.; Breuker, H.; Camporesi, T.; Castello, R.; Cepeda, M.; Cerminara, G.; D'Alfonso, M.; d'Enterria, D.; Dabrowski, A.; Daponte, V.; David, A.; De Gruttola, M.; De Guio, F.; De Roeck, A.; Di Marco, E.; Dobson, M.; Dordevic, M.; Dorney, B.; du Pree, T.; Duggan, D.; Dunser, M.; Dupont, N.; Elliott-Peisert, A.; Fartoukh, S.; Franzoni, G.; Fulcher, J.; Funk, W.; Gigi, D.; Gill, K.; Girone, M.; Glege, F.; Guida, R.; Gundacker, S.; Guthoff, M.; Hammer, J.; Harris, P.; Hegeman, J.; Innocente, V.; Janot, P.; Kirschenmann, H.; Knunz, V.; Kortelainen, M. J.; Kousouris, K.; Lecoq, P.; Lourenco, C.; Lucchini, M. T.; Magini, N.; Malgeri, L.; Mannelli, M.; Martelli, A.; Masetti, L.; Meijers, F.; Mersi, S.; Meschi, E.; Moortgat, F.; Morovic, S.; Mulders, M.; Neugebauer, H.; Orfanelli, S.; Orsini, L.; Pape, L.; Perez, E.; Peruzzi, M.; Petrilli, A.; Petrucciani, G.; Pfeiffer, A.; Pierini, M.; Piparo, D.; Racz, A.; Reis, T.; Rolandi, G.; Rovere, M.; Ruan, M.; Sakulin, H.; Sauvan, J. B.; Schafer, C.; Schwick, C.; Seidel, M.; Sharma, A.; Silva, P.; Simon, M.; Sphicas, P.; Steggemann, J.; Stoye, M.; Takahashi, Y.; Treille, D.; Triossi, A.; Tsirou, A.; Veckalns, V.; Veres, G. I.; Wardle, N.; Wohri, H. K.; Zagozdzinska, A.; Zeuner, W. D.] CERN, European Org Nucl Res, Geneva, Switzerland.
[Bertl, W.; Deiters, K.; Erdmann, W.; Horisberger, R.; Ingram, Q.; Kaestli, H. C.; Kotlinski, D.; Langenegger, U.; Rohe, T.] Paul Scherrer Inst, Villigen, Switzerland.
[Bachmair, F.; Bani, L.; Bianchini, L.; Casal, B.; Dissertori, G.; Dittmar, M.; Donega, M.; Eller, P.; Grab, C.; Heidegger, C.; Hits, D.; Hoss, J.; Kasieczka, G.; Lecomte, P.; Lustermann, W.; Mangano, B.; Marionneau, M.; del Arbol, P. Martinez Ruiz; Masciovecchio, M.; Meinhard, M. T.; Meister, D.; Micheli, F.; Musella, P.; Nessi-Tedaldi, F.; Pandolfi, F.; Pata, J.; Pauss, F.; Perrin, G.; Perrozzi, L.; Quittnat, M.; Rossini, M.; Schonenberger, M.; Starodumov, A.; Takahashi, M.; Tavolaro, V. R.; Theofilatos, K.; Wallny, R.] Swiss Fed Inst Technol, Inst Particle Phys, Zurich, Switzerland.
[Aarrestad, T. K.; Amsler, C.; Caminada, L.; Canelli, M. F.; Chiochia, V.; De Cosa, A.; Galloni, C.; Hinzmann, A.; Hreus, T.; Kilminster, B.; Lange, C.; Ngadiuba, J.; Pinna, D.; Rauco, G.; Robmann, P.; Salerno, D.; Yang, Y.] Univ Zurich, Zurich, Switzerland.
[Chen, K. H.; Doan, T. H.; Jain, Sh.; Khurana, R.; Konyushikhin, M.; Kuo, C. M.; Lin, W.; Lu, Y. J.; Pozdnyakov, A.; Yu, S. S.] Natl Cent Univ, Chungli, Taiwan.
[Kumar, Arun; Chang, P.; Chang, Y. H.; Chang, Y. W.; Chao, Y.; Chen, K. F.; Chen, P. H.; Dietz, C.; Fiori, F.; Hou, W. -S.; Hsiung, Y.; Liu, Y. F.; Lu, R. -S.; Moya, M. Minano; Tsai, J. F.; Tzeng, Y. M.] NTU, Taipei, Taiwan.
[Asavapibhop, B.; Kovitanggoon, K.; Singh, G.; Srimanobhas, N.; Suwonjandee, N.] Chulalongkorn Univ, Fac Sci, Dept Phys, Bangkok, Thailand.
[Adiguzel, A.; Cerci, S.; Damarseckin, S.; Demiroglu, Z. S.; Dozen, C.; Dumanoglu, I.; Girgis, S.; Gokbulut, G.; Guler, Y.; Gurpinar, E.; Hos, I.; Kangal, E. E.; Topaksu, A. Kayis; Onengut, G.; Ozdemir, K.; Ozturk, S.; Tali, B.; Topakli, H.; Zorbilmez, C.] Cukurova Univ, Adana, Turkey.
[Bilin, B.; Bilmis, S.; Isildak, B.; Karapinar, G.; Yalvac, M.; Zeyrek, M.] Middle East Tech Univ, Dept Phys, Ankara, Turkey.
[Gulmez, E.; Kaya, M.; Kaya, O.; Yetkin, E. A.; Yetkin, T.] Bogazici Univ, Istanbul, Turkey.
[Cakir, A.; Cankocak, K.; Sen, S.; Vardarli, F. I.] Istanbul Tech Univ, Istanbul, Turkey.
[Grynyov, B.] Natl Acad Sci Ukraine, Inst Scintillat Mat, Kharkov, Ukraine.
[Levchuk, L.; Sorokin, P.] Kharkov Inst Phys & Technol, Natl Sci Ctr, Kharkov, Ukraine.
[Aggleton, R.; Ball, F.; Beck, L.; Brooke, J. J.; Burns, D.; Clement, E.; Cussans, D.; Flacher, H.; Goldstein, J.; Grimes, M.; Heath, G. P.; Heath, H. F.; Jacob, J.; Kreczko, L.; Lucas, C.; Meng, Z.; Newbold, D. M.; Paramesvaran, S.; Poll, A.; Sakuma, T.; El Nasr-Storey, S. Seif; Senkin, S.; Smith, D.; Smith, V. J.] Univ Bristol, Bristol, Avon, England.
[Bell, K. W.; Belyaev, A.; Brew, C.; Brown, R. M.; Calligaris, L.; Cieri, D.; Cockerill, D. J. A.; Coughlan, J. A.; Harder, K.; Harper, S.; Olaiya, E.; Petyt, D.; Shepherd-Themistocleous, C. H.; Thea, A.; Tomalin, I. R.; Williams, T.; Worm, S. D.] Rutherford Appleton Lab, Didcot, Oxon, England.
[Baber, M.; Bainbridge, R.; Buchmuller, O.; Bundock, A.; Burton, D.; Casasso, S.; Citron, M.; Colling, D.; Corpe, L.; Dauncey, P.; Davies, G.; De Wit, A.; Della Negra, M.; Dunne, P.; Elwood, A.; Futyan, D.; Haddad, Y.; Hall, G.; Iles, G.; Lane, R.; Lucas, R.; Lyons, L.; Magnan, A. -M.; Malik, S.; Mastrolorenzo, L.; Nash, J.; Nikitenko, A.; Pela, J.; Penning, B.; Pesaresi, M.; Raymond, D. M.; Richards, A.; Rose, A.; Seez, C.; Tapper, A.; Uchida, K.; Acosta, M. Vazquez; Virdee, T.; Zenz, S. C.] Imperial Coll, London, England.
[Cole, J. E.; Hobson, P. R.; Khan, A.; Kyberd, P.; Leslie, D.; Reid, I. D.; Symonds, P.; Teodorescu, L.; Turner, M.] Brunel Univ, Uxbridge, Middx, England.
[Borzou, A.; Call, K.; Dittmann, J.; Hatakeyama, K.; Liu, H.; Pastika, N.] Baylor Univ, Waco, TX 76798 USA.
[Charaf, O.; Cooper, S. I.; Henderson, C.; Rumerio, P.] Univ Alabama, Tuscaloosa, AL USA.
[Arcaro, D.; Avetisyan, A.; Bose, T.; Gastler, D.; Rankin, D.; Richardson, C.; Rohlf, J.; Sulak, L.; Zou, D.] Boston Univ, Boston, MA 02215 USA.
[Alimena, J.; Benelli, G.; Berry, E.; Cutts, D.; Ferapontov, A.; Garabedian, A.; Hakala, J.; Heintz, U.; Jesus, O.; Laird, E.; Landsberg, G.; Mao, Z.; Narain, M.; Piperov, S.; Sagir, S.; Syarif, R.] Brown Univ, Providence, RI 02912 USA.
[Breedon, R.; Breto, G.; Sanchez, M. Calderon De la Barca; Chauhan, S.; Chertok, M.; Conway, J.; Conway, R.; Cox, P. T.; Erbacher, R.; Funk, G.; Gardner, M.; Ko, W.; Lander, R.; Mclean, C.; Mulhearn, M.; Pellett, D.; Pilot, J.; Ricci-Tam, F.; Shalhout, S.; Smith, J.; Squires, M.; Stolp, D.; Tripathi, M.; Wilbur, S.; Yohay, R.] Univ Calif Davis, Davis, CA 95616 USA.
[Cousins, R.; Everaerts, P.; Florent, A.; Hauser, J.; Ignatenko, M.; Saltzberg, D.; Takasugi, E.; Valuev, V.; Weber, M.] Univ Calif Los Angeles, Los Angeles, CA USA.
[Burt, K.; Clare, R.; Ellison, J.; Gary, J. W.; Hanson, G.; Heilman, J.; Paneva, M. Ivova; Jandir, P.; Kennedy, E.; Lacroix, F.; Long, O. R.; Malberti, M.; Negrete, M. Olmedo; Shrinivas, A.; Wei, H.; Wimpenny, S.; Yates, B. R.] Univ Calif Riverside, Riverside, CA 92521 USA.
[Branson, J. G.; Cerati, G. B.; Cittolin, S.; D'Agnolo, R. T.; Derdzinski, M.; Gerosa, R.; Holzner, A.; Kelley, R.; Klein, D.; Letts, J.; Macneill, I.; Olivito, D.; Padhi, S.; Pieri, M.; Sani, M.; Sharma, V.; Simon, S.; Tadel, M.; Vartak, A.; Wasserbaech, S.; Welke, C.; Wood, J.; Wurthwein, F.; Yagil, A.; Della Porta, G. Zevi] Univ Calif San Diego, La Jolla, CA 92093 USA.
[Bradmiller-Feld, J.; Campagnari, C.; Dishaw, A.; Dutta, V.; Flowers, K.; Sevilla, M. Franco; Geffert, P.; George, C.; Golf, F.; Gouskos, L.; Gran, J.; Incandela, J.; Mccoll, N.; Mullin, S. D.; Richman, J.; Stuart, D.; Suarez, I.; West, C.; Yoo, J.] Univ Calif Santa Barbara, Santa Barbara, CA 93106 USA.
[Anderson, D.; Apresyan, A.; Bendavid, J.; Bornheim, A.; Bunn, J.; Chen, Y.; Duarte, J.; Mott, A.; Newman, H. B.; Pena, C.; Spiropulu, M.; Vlimant, J. R.; Xie, S.; Zhu, R. Y.] CALTECH, Pasadena, CA 91125 USA.
[Andrews, M. B.; Azzolini, V.; Calamba, A.; Carlson, B.; Ferguson, T.; Paulini, M.; Russ, J.; Sun, M.; Vogel, H.; Vorobiev, I.] Carnegie Mellon Univ, Pittsburgh, PA 15213 USA.
[Cumalat, J. P.; Ford, W. T.; Jensen, F.; Johnson, A.; Krohn, M.; Mulholland, T.; Nauenberg, U.; Stenson, K.; Wagner, S. R.] Univ Colorado Boulder, Boulder, CO USA.
[Alexander, J.; Chatterjee, A.; Chaves, J.; Chu, J.; Dittmer, S.; Eggert, N.; Mirman, N.; Kaufman, G. Nicolas; Patterson, J. R.; Rinkevicius, A.; Ryd, A.; Skinnari, L.; Soffi, L.; Sun, W.; Tan, S. M.; Teo, W. D.; Thom, J.; Thompson, J.; Tucker, J.; Weng, Y.; Wittich, P.] Cornell Univ, Ithaca, NY USA.
[Abdullin, S.; Albrow, M.; Apollinari, G.; Banerjee, S.; Bauerdick, L. A. T.; Beretvas, A.; Berryhill, J.; Bhat, P. C.; Bolla, G.; Burkett, K.; Butler, J. N.; Cheung, H. W. K.; Chlebana, F.; Cihangir, S.; Elvira, V. D.; Fisk, I.; Freeman, J.; Gottschalk, E.; Gray, L.; Green, D.; Grunendahl, S.; Gutsche, O.; Hanlon, J.; Hare, D.; Harris, R. M.; Hasegawa, S.; Hirschauer, J.; Hu, Z.; Jayatilaka, B.; Jindariani, S.; Johnson, M.; Joshi, U.; Klima, B.; Kreis, B.; Lammel, S.; Lewis, J.; Linacre, J.; Lincoln, D.; Lipton, R.; Liu, T.; De Sa, R. Lopes; Lykken, J.; Maeshima, K.; Marraffino, J. M.; Maruyama, S.; Mason, D.; McBride, P.; Merkel, P.; Mrenna, S.; Nahn, S.; Newman-Holmes, C.; O'Dell, V.; Pedro, K.; Prokofyev, O.; Rakness, G.; Sexton-Kennedy, E.; Soha, A.; Spalding, W. J.; Spiegel, L.; Stoynev, S.; Strobbe, N.; Taylor, L.; Tkaczyk, S.; Tran, N. V.; Uplegger, L.; Vaandering, E. W.; Vernieri, C.; Verzocchi, M.; Vidal, R.; Wang, M.; Weber, H. A.; Whitbeck, A.] Fermilab Natl Accelerator Lab, POB 500, Batavia, IL 60510 USA.
[Acosta, D.; Bourilkov, D.; Brinkerhoff, A.; Carnes, A.; Curry, D.; Furic, I. K.; Konigsberg, J.; Korytov, A.; Kotov, K.; Mei, H.; Mitselmakher, G.; Rank, D.; Sperka, D.; Wang, J.; Yelton, J.] Univ Florida, Gainesville, FL USA.
[Linn, S.; Markowitz, P.; Martinez, G.; Rodriguez, J. L.] Florida Int Univ, Miami, FL 33199 USA.
[Ackert, A.; Adams, J. R.; Adams, T.; Askew, A.; Bein, S.; Bochenek, J.; Diamond, B.; Haas, J.; Hagopian, S.; Hagopian, V.; Johnson, K. F.; Khatiwada, A.; Prosper, H.; Santra, A.; Weinberg, M.] Florida State Univ, Tallahassee, FL 32306 USA.
[Baarmand, M. M.; Bhopatkar, V.; Colafranceschi, S.; Hohlmann, M.; Kalakhety, H.; Noonan, D.; Roy, T.; Yumiceva, F.] Florida Inst Technol, Melbourne, FL 32901 USA.
[Adams, M. R.; Apanasevich, L.; Berry, D.; Betts, R. R.; Bucinskaite, I.; Cavanaugh, R.; Evdokimov, O.; Gauthier, L.; Gerber, C. E.; Hofman, D. J.; Kurt, P.; O'Brien, C.; Gonzalez, I. D. Sandoval; Turner, P.; Varelas, N.; Wu, Z.; Zakaria, M.; Zhang, J.; Bilki, B.] UIC, Chicago, IL USA.
[Clarida, W.; Dilsiz, K.; Durgut, S.; Gandrajula, R. P.; Haytmyradov, M.; Khristenko, V.; Merlo, J. -P.; Mermerkaya, H.; Mestvirishvili, A.; Moeller, A.; Nachtman, J.; Ogul, H.; Onel, Y.; Ozok, F.; Penzo, A.; Snyder, C.; Tiras, E.; Wetzel, J.; Yi, K.] Univ Iowa, Iowa City, IA USA.
[Anderson, I.; Blumenfeld, B.; Cocoros, A.; Eminizer, N.; Fehling, D.; Feng, L.; Gritsan, A. V.; Maksimovic, P.; Osherson, M.; Roskes, J.; Sarica, U.; Swartz, M.; Xiao, M.; Xin, Y.; You, C.] Johns Hopkins Univ, Baltimore, MD USA.
[Baringer, P.; Bean, A.; Bruner, C.; Castle, J.; Kenny, R. P., III; Kropivnitskaya, A.; Majumder, D.; Malek, M.; Mcbrayer, W.; Murray, M.; Sanders, S.; Stringer, R.; Wang, Q.] Univ Kansas, Lawrence, KS 66045 USA.
[Ivanov, A.; Kaadze, K.; Khalil, S.; Makouski, M.; Maravin, Y.; Mohammadi, A.; Saini, L. K.; Skhirtladze, N.; Toda, S.] Kansas State Univ, Manhattan, KS 66506 USA.
[Lange, D.; Rebassoo, F.; Wright, D.] Lawrence Livermore Natl Lab, Livermore, CA USA.
[Anelli, C.; Baden, A.; Baron, O.; Belloni, A.; Calvert, B.; Eno, S. C.; Ferraioli, C.; Gomez, J. A.; Hadley, N. J.; Jabeen, S.; Kellogg, R. G.; Kolberg, T.; Kunkle, J.; Lu, Y.; Mignerey, A. C.; Shin, Y. H.; Skuja, A.; Tonjes, M. B.; Tonwar, S. C.] Univ Maryland, College Pk, MD 20742 USA.
[Apyan, A.; Barbieri, R.; Baty, A.; Bi, R.; Bierwagen, K.; Brandt, S.; Busza, W.; Cali, I. A.; Demiragli, Z.; Di Matteo, L.; Ceballos, G. Gomez; Goncharov, M.; Gulhan, D.; Hsu, D.; Iiyama, Y.; Innocenti, G. M.; Klute, M.; Kovalskyi, D.; Krajczar, K.; Lai, Y. S.; Lee, Y. -J.; Levin, A.; Luckey, P. D.; Marini, A. C.; Mcginn, C.; Mironov, C.; Narayanan, S.; Niu, X.; Paus, C.; Roland, C.; Roland, G.; Salfeld-Nebgen, J.; Stephans, G. S. F.; Sumorok, K.; Tatar, K.; Varma, M.; Velicanu, D.; Veverka, J.; Wang, J.; Wang, T. W.; Wyslouch, B.; Yang, M.; Zhukova, V.] MIT, 77 Massachusetts Ave, Cambridge, MA 02139 USA.
[Benvenuti, A. C.; Dahmes, B.; Evans, A.; Finkel, A.; Gude, A.; Hansen, P.; Kalafut, S.; Kao, S. C.; Klapoetke, K.; Kubota, Y.; Lesko, Z.; Mans, J.; Nourbakhsh, S.; Ruckstuhl, N.; Rusack, R.; Tambe, N.; Turkewitz, J.] Univ Minnesota, Minneapolis, MN USA.
[Acosta, J. G.; Oliveros, S.] Univ Mississippi, Oxford, MS USA.
[Avdeeva, E.; Bartek, R.; Bloom, K.; Bose, S.; Claes, D. R.; Dominguez, A.; Fangmeier, C.; Suarez, R. Gonzalez; Kamalieddin, R.; Knowlton, D.; Kravchenko, I.; Meier, F.; Monroy, J.; Ratnikov, F.; Siado, J. E.; Snow, G. R.; Stieger, B.] Univ Nebraska, Lincoln, NE USA.
[Alyari, M.; Dolen, J.; George, J.; Godshalk, A.; Harrington, C.; Iashvili, I.; Kaisen, J.; Kharchilava, A.; Kumar, A.; Parker, A.; Rappoccio, S.; Roozbahani, B.] SUNY Buffalo, Buffalo, NY USA.
[Alverson, G.; Barberis, E.; Baumgartel, D.; Chasco, M.; Hortiangtham, A.; Massironi, A.; Morse, D. M.; Nash, D.; Orimoto, T.; De Lima, R. Teixeira; Trocino, D.; Wang, R. -J.; Wood, D.; Zhang, J.] Northeastern Univ, Boston, MA 02115 USA.
[Bhattacharya, S.; Hahn, K. A.; Kubik, A.; Low, J. F.; Mucia, N.; Odell, N.; Pollack, B.; Schmitt, M. H.; Sung, K.; Trovato, M.; Velasco, M.] Northwestern Univ, Evanston, IL USA.
[Dev, N.; Hildreth, M.; Jessop, C.; Karmgard, D. J.; Kellams, N.; Lannon, K.; Marinelli, N.; Meng, F.; Mueller, C.; Musienko, Y.; Planer, M.; Reinsvold, A.; Ruchti, R.; Rupprecht, N.; Smith, G.; Taroni, S.; Valls, N.; Wayne, M.; Wolf, M.; Woodard, A.] Univ Notre Dame, Notre Dame, IN 46556 USA.
[Antonelli, L.; Brinson, J.; Bylsma, B.; Durkin, L. S.; Flowers, S.; Hart, A.; Hill, C.; Hughes, R.; Ji, W.; Ling, T. Y.; Liu, B.; Luo, W.; Puigh, D.; Rodenburg, M.; Winer, B. L.; Wulsin, H. W.] Ohio State Univ, Columbus, OH 43210 USA.
[Driga, O.; Elmer, P.; Hardenbrook, J.; Hebda, P.; Koay, S. A.; Lujan, P.; Marlow, D.; Medvedeva, T.; Mooney, M.; Olsen, J.; Palmer, C.; Piroue, P.; Stickland, D.; Tully, C.; Zuranski, A.] Princeton Univ, Princeton, NJ 08544 USA.
[Malik, S.] Univ Puerto Rico, Mayaguez, PR USA.
[Barker, A.; Barnes, V. E.; Benedetti, D.; Gutay, L.; Jha, M. K.; Jones, M.; Jung, A. W.; Jung, K.; Miller, D. H.; Neumeister, N.; Radburn-Smith, B. C.; Shi, X.; Sun, J.; Svyatkovskiy, A.; Wang, F.; Xie, W.; Xu, L.] Purdue Univ, W Lafayette, IN 47907 USA.
[Parashar, N.; Stupak, J.] Purdue Univ Calumet, Hammond, IN USA.
[Adair, A.; Akgun, B.; Chen, Z.; Ecklund, K. M.; Geurts, F. J. M.; Guilbaud, M.; Li, W.; Michlin, B.; Northup, M.; Padley, B. P.; Redjimi, R.; Roberts, J.; Rorie, J.; Tu, Z.; Zabel, J.] Rice Univ, Houston, TX USA.
[Betchart, B.; Bodek, A.; de Barbaro, P.; Demina, R.; Duh, Y. T.; Eshaq, Y.; Ferbel, T.; Galanti, M.; Garcia-Bellido, A.; Han, J.; Hindrichs, O.; Khukhunaishvili, A.; Lo, K. H.; Tan, P.; Verzetti, M.] Univ Rochester, Rochester, NY USA.
[Chou, J. P.; Contreras-Campana, E.; Gershtein, Y.; Espinosa, T. A. Gomez; Halkiadakis, E.; Heindl, M.; Hidas, D.; Hughes, E.; Kaplan, S.; Elayavalli, R. Kunnawalkam; Kyriacou, S.; Lath, A.; Nash, K.; Saka, H.; Salur, S.; Schnetzer, S.; Sheffield, D.; Somalwar, S.; Stone, R.; Thomas, S.; Thomassen, P.; Walker, M.] Rutgers State Univ, Piscataway, NJ USA.
[Foerster, M.; Heideman, J.; Riley, G.; Rose, K.; Spanier, S.; Thapa, K.] Univ Tennessee, Knoxville, TN USA.
[Bouhali, O.; Hernandez, A. Castaneda; Celik, A.; Dalchenko, M.; De Mattia, M.; Delgado, A.; Dildick, S.; Eusebi, R.; Gilmore, J.; Huang, T.; Kamon, T.; Krutelyov, V.; Mueller, R.; Osipenkov, I.; Pakhotin, Y.; Patel, R.; Perloff, A.; Pernie, L.; Rathjens, D.; Rose, A.; Safonov, A.; Tatarinov, A.; Ulmer, K. A.] Texas A&M Univ, College Stn, TX USA.
[Akchurin, N.; Cowden, C.; Damgov, J.; Dragoiu, C.; Dudero, P. R.; Faulkner, J.; Kunori, S.; Lamichhane, K.; Lee, S. W.; Libeiro, T.; Undleeb, S.; Volobouev, I.; Wang, Z.] Texas Tech Univ, Lubbock, TX 79409 USA.
[Appelt, E.; Delannoy, A. G.; Greene, S.; Gurrola, A.; Janjam, R.; Johns, W.; Maguire, C.; Mao, Y.; Melo, A.; Ni, H.; Sheldon, P.; Tuo, S.; Velkovska, J.; Xu, Q.] Vanderbilt Univ, 221 Kirkland Hall, Nashville, TN 37235 USA.
[Arenton, M. W.; Barria, P.; Cox, B.; Francis, B.; Goodell, J.; Hirosky, R.; Ledovskoy, A.; Li, H.; Neu, C.; Sinthuprasith, T.; Sun, X.; Wang, Y.; Wolfe, E.; Xia, F.] Univ Virginia, Charlottesville, VA USA.
[Clarke, C.; Harr, R.; Karchin, P. E.; Don, C. Kottachchi Kankanamge; Lamichhane, P.; Sturdy, J.] Wayne State Univ, Detroit, MI USA.
[Belknap, D. A.; Carlsmith, D.; Dasu, S.; Dodd, L.; Duric, S.; Gomber, B.; Grothe, M.; Herndon, M.; Herve, A.; Klabbers, P.; Lanaro, A.; Levine, A.; Long, K.; Loveless, R.; Mohapatra, A.; Ojalvo, I.; Perry, T.; Pierro, G. A.; Polese, G.; Ruggles, T.; Sarangi, T.; Savin, A.; Sharma, A.; Smith, N.; Smith, W. H.; Taylor, D.; Verwilligen, P.; Woods, N.] Univ Wisconsin, Madison, WI USA.
[Fruhwirth, R.; Jeitler, M.; Krammer, M.; Schieck, J.; Wulz, C. -E.] Vienna Univ Technol, Vienna, Austria.
Peking Univ, State Key Lab Nucl Phys & Technol, Beijing, Peoples R China.
[Beluffi, C.] Univ Strasbourg, Inst Pluridisciplinaire Hubert Curien, Univ Haute Alsace Mulhouse, CNRS,IN2P3, Strasbourg, France.
[Chinellato, J.; Manganote, E. J. Tonelli] Univ Estadual Campinas, Campinas, SP, Brazil.
[Moon, C. S.] CNRS, IN2P3, Paris, France.
[Fang, W.] Univ Libre Bruxelles, Brussels, Belgium.
[Plestina, R.] Ecole Polytech, CNRS, IN2P3, Lab Leprince Ringuet, Palaiseau, France.
[Finger, M.; Finger, M., Jr.; Tsamalaidze, Z.] Joint Inst Nucl Res, Dubna, Russia.
[Assran, Y.] Suez Univ, Suez, Egypt.
[Assran, Y.; Radi, A.] British Univ Egypt, Cairo, Egypt.
[Kamel, A. Ellithi] Cairo Univ, Cairo, Egypt.
[Mahrous, A.] Helwan Univ, Cairo, Egypt.
[Radi, A.] Ain Shams Univ, Cairo, Egypt.
[Agram, J. -L.; Conte, E.; Fontaine, J. -C.] Univ Haute Alsace, Mulhouse, France.
[Merlin, J. A.; Stahl, A.; Pantaleo, F.; Hartmann, F.; Kornmayer, A.; Mohanty, A. K.; Silvestris, L.; Tosi, N.; Viliani, L.; Primavera, F.; Manzoni, R. A.; Di Guida, S.; Meola, S.; Paolucci, P.; Azzi, P.; Pazzini, J.; Azzurri, P.; D'imperio, G.; Del Re, D.; Arcidiacono, R.; Virdee, T.] CERN, European Org Nucl Res, Geneva, Switzerland.
[Popov, A.; Zhukov, V.; Katkov, I.] Lomonosov Moscow State Univ, Skobeltsyn Inst Nucl Phys, Moscow, Russia.
[Toriashvili, T.] Tbilisi State Univ, Tbilisi, Rep of Georgia.
[Borras, K.] Rhein Westfal TH Aachen, Phys Inst A3, Aachen, Germany.
[Gallo, E.] Univ Hamburg, Hamburg, Germany.
[Hempel, M.; Karacheban, O.; Lohmann, W.] Brandenburg Tech Univ Cottbus, Cottbus, Germany.
[Horvath, D.] Inst Nucl Res ATOMKI, Debrecen, Hungary.
[Vesztergombi, G.; Bartok, M.; Veres, G. I.] Eotvos Lorand Univ, MTA ELTE Lendulet CMS Particle & Nucl Phys Grp, Budapest, Hungary.
[Karancsi, J.] Univ Debrecen, Debrecen, Hungary.
[Choudhury, S.] Indian Inst Sci Educ & Res, Bhopal, India.
[Bhowmik, S.; Maity, M.; Sarkar, T.] Visva Bharati Univ, Santini Ketan, W Bengal, India.
[Gurtu, A.] King Abdulaziz Univ, Jeddah, Saudi Arabia.
[Wickramage, N.] Univ Ruhuna, Matara, Sri Lanka.
[Etesami, S. M.] Isfahan Univ Technol, Esfahan, Iran.
[Fahim, A.] Univ Tehran, Dept Engn Sci, Tehran, Iran.
Islamic Azad Univ, Sci & Res Branch, Plasma Phys Res Ctr, Tehran, Iran.
[Androsov, K.; Ciocci, M. A.; Grippo, M. T.] Univ Siena, Siena, Italy.
[Savoy-Navarro, A.] Purdue Univ, W Lafayette, IN 47907 USA.
[Kim, T. J.] Hanyang Univ, Seoul, South Korea.
[Ali, M. A. B. Md] Int Islamic Univ Malaysia, Kuala Lumpur, Malaysia.
[Idris, F. Mohamad] MOSTI, Malaysian Nucl Agcy, Kajang, Malaysia.
[Heredia-De La Cruz, I.] Consejo Nacl Ciencia & Technol, Mexico City, DF, Mexico.
[Byszuk, A.; Zagozdzinska, A.] Warsaw Univ Technol, Inst Elect Syst, Warsaw, Poland.
[Matveev, V.; Musienko, Y.] Inst Nucl Res, Moscow, Russia.
[Matveev, V.; Azarkin, M.; Dremin, I.; Leonidov, A.] Natl Res Nucl Univ, Moscow Engn Phys Inst MEPhI, Moscow, Russia.
[Kim, V.] St Petersburg State Polytech Univ, St Petersburg, Russia.
[Kuznetsova, E.] Univ Florida, Gainesville, FL USA.
[Dubinin, M.] CALTECH, Pasadena, CA 91125 USA.
[Adzic, P.] Univ Belgrade, Fac Phys, Belgrade, Serbia.
[Dobson, M.] Univ Rome, Ist Nazl Fis Nucl, Sez Roma, Rome, Italy.
[Orfanelli, S.] Natl Tech Univ Athens, Athens, Greece.
[Rolandi, G.] Scuola Normale, Pisa, Italy.
[Rolandi, G.] Sezione Ist Nazl Fis Nucl, Pisa, Italy.
[Sphicas, P.] Univ Athens, Athens, Greece.
[Veckalns, V.] Riga Tech Univ, Riga, Latvia.
[Starodumov, A.; Nikitenko, A.] Inst Theoret & Expt Phys, Moscow, Russia.
[Amsler, C.] Albert Einstein Ctr Fundamental Phys, Bern, Switzerland.
[Cerci, S.; Tali, B.] Adiyaman Univ, Adiyaman, Turkey.
[Kangal, E. E.] Mersin Univ, Mersin, Turkey.
[Onengut, G.] Cag Univ, Mersin, Turkey.
[Ozdemir, K.] Piri Reis Univ, Istanbul, Turkey.
[Ozturk, S.; Topakli, H.] Gaziosmanpasa Univ, Tokat, Turkey.
[Isildak, B.] Ozyegin Univ, Istanbul, Turkey.
[Karapinar, G.] Izmir Inst Technol, Izmir, Turkey.
[Kaya, M.] Marmara Univ, Istanbul, Turkey.
[Kaya, O.] Kafkas Univ, Kars, Turkey.
[Yetkin, E. A.] Istanbul Bilgi Univ, Istanbul, Turkey.
[Yetkin, T.] Yildiz Tech Univ, Istanbul, Turkey.
[Sen, S.] Hacettepe Univ, Ankara, Turkey.
[Newbold, D. M.; Lucas, R.] Rutherford Appleton Lab, Didcot, Oxon, England.
[Belyaev, A.] Univ Southampton, Sch Phys & Astron, Southampton, Hants, England.
[Acosta, M. Vazquez] Inst Astrofis Canarias, San Cristobal la Laguna, Spain.
[Wasserbaech, S.] Utah Valley Univ, Orem, UT USA.
[Milenovic, P.] Univ Belgrade, Fac Phys, Belgrade, Serbia.
[Milenovic, P.] Vinca Inst Nucl Sci, Belgrade, Serbia.
[Colafranceschi, S.] Univ Roma, Fac Ingn, Rome, Italy.
[Bilki, B.] Argonne Natl Lab, 9700 S Cass Ave, Argonne, IL 60439 USA.
[Mermerkaya, H.] Erzincan Univ, Erzincan, Turkey.
[Ozok, F.] Mimar Sinan Univ, Istanbul, Turkey.
[Bouhali, O.; Hernandez, A. Castaneda] Texas A&M Univ Qatar, Doha, Qatar.
[Kamon, T.] Kyungpook Natl Univ, Daegu, South Korea.
RP Khachatryan, V (reprint author), Yerevan Phys Inst, Yerevan, Armenia.
RI Azarkin, Maxim/N-2578-2015; Danilov, Mikhail/C-5380-2014; Kirakosyan,
Martin/N-2701-2015; Della Ricca, Giuseppe/B-6826-2013; Puljak,
Ivica/D-8917-2017; TUVE', Cristina/P-3933-2015; Goh,
Junghwan/Q-3720-2016; Manganote, Edmilson/K-8251-2013; Dremin,
Igor/K-8053-2015; Lokhtin, Igor/D-7004-2012; Yazgan, Efe/C-4521-2014;
Konecki, Marcin/G-4164-2015; Chistov, Ruslan/B-4893-2014; Leonidov,
Andrey/M-4440-2013; Paulini, Manfred/N-7794-2014; Andreev,
Vladimir/M-8665-2015; Chadeeva, Marina/C-8789-2016; Smirnov,
Vitaly/B-5001-2017; Moraes, Arthur/F-6478-2010; Ogul, Hasan/S-7951-2016
OI Danilov, Mikhail/0000-0001-9227-5164; Della Ricca,
Giuseppe/0000-0003-2831-6982; TUVE', Cristina/0000-0003-0739-3153; Goh,
Junghwan/0000-0002-1129-2083; Yazgan, Efe/0000-0001-5732-7950; Konecki,
Marcin/0000-0001-9482-4841; Chistov, Ruslan/0000-0003-1439-8390;
Paulini, Manfred/0000-0002-6714-5787; Chadeeva,
Marina/0000-0003-1814-1218; Moraes, Arthur/0000-0002-5157-5686; Ogul,
Hasan/0000-0002-5121-2893
FU Austrian Federal Ministry of Science, Research and Economy; Austrian
Science Fund; Belgian Fonds de la Recherche Scientifique; Fonds voor
Wetenschappelijk Onderzoek; Brazilian Funding Agency (CNPq); Brazilian
Funding Agency (CAPES); Brazilian Funding Agency (FAPERJ); Brazilian
Funding Agency (FAPESP); Bulgarian Ministry of Education and Science;
CERN; Chinese Academy of Sciences; National Natural Science Foundation
of China; Colombian Funding Agency (COLCIENCIAS); Croatian Ministry of
Science, Education and Sport; Croatian Science Foundation; Research
Promotion Foundation, Cyprus; Ministry of Education and Research;
Estonian Research Council [IUT23-4, IUT23-6]; European Regional
Development Fund, Estonia; Academy of Finland; Finnish Ministry of
Education and Culture; Helsinki Institute of Physics; Institut National
de Physique Nucleaire et de Physique des Particules / CNRS; Commissariat
a l'Energie Atomique et aux Energies Alternatives / CEA, France;
Bundesministerium fur Bildung und Forschung; Deutsche
Forschungsgemeinschaft; Helmholtz-Gemeinschaft Deutscher
Forschungszentren, Germany; General Secretariat for Research and
Technology, Greece; National Scientific Research Foundation; National
Innovation Office, Hungary; Department of Atomic Energy; Department of
Science and Technology, India; Institute for Studies in Theoretical
Physics and Mathematics, Iran; Science Foundation, Ireland; Istituto
Nazionale di Fisica Nucleare, Italy; Ministry of Science, ICT and Future
Planning; National Research Foundation (NRF), Republic of Korea;
Lithuanian Academy of Sciences; Ministry of Education; University of
Malaya (Malaysia); Mexican Funding Agency (BUAP); Mexican Funding Agency
(CINVESTAV); Mexican Funding Agency (CONACYT); Mexican Funding Agency
(LNS); Mexican Funding Agency (SEP); Mexican Funding Agency (UASLP-FAI);
Ministry of Business, Innovation and Employment, New Zealand; Pakistan
Atomic Energy Commission; Ministry of Science and Higher Education;
National Science Center, Poland; Fundacao para a Ciencia e a Tecnologia,
Portugal; JINR, Dubna; Ministry of Education and Science of the Russian
Federation; Federal Agency of Atomic Energy of the Russian Federation;
Russian Academy of Sciences; Russian Foundation for Basic Research;
Ministry of Education, Science and Technological Development of Serbia;
Secretaria de Estado de Investigacion, Spain; Desarrollo e Innovacion,
Spain; Programa Consolider-Ingenio, Spain; Swiss Funding Agency (ETH
Board); Swiss Funding Agency (ETH Zurich); Swiss Funding Agency (PSI);
Swiss Funding Agency (SNF); Swiss Funding Agency (UniZH); Swiss Funding
Agency (Canton Zurich); Swiss Funding Agency (SER); Ministry of Science
and Technology, Taipei; Thailand Center of Excellence in Physics, the
Institute for the Promotion of Teaching Science and Technology of
Thailand; Special Task Force for Activating Research; National Science
and Technology Development Agency of Thailand; Scientific and Technical
Research Council of Turkey; Turkish Atomic Energy Authority; National
Academy of Sciences of Ukraine; State Fund for Fundamental Researches,
Ukraine; Science and Technology Facilities Council, UK; US Department of
Energy; US National Science Foundation; Marie-Curie program; European
Research Council; EPLANET; Leventis Foundation; A. P. Sloan Foundation;
Alexander von Humboldt Foundation; Belgian Federal Science Policy
Office; Fonds pour la Formation a la Recherche dans l'Industrie et dans
l'Agriculture (FRIA-Belgium); Agentschap voor Innovatie door Wetenschap
en Technologie (IWT-Belgium); Ministry of Education, Youth and Sports
(MEYS) of the Czech Republic; Council of Science and Industrial
Research, India; HOMING PLUS program of the Foundation for Polish
Science; European Union, Regional Development Fund; Mobility Plus
program of the Ministry of Science and Higher Education (Poland); OPUS
program of the National Science Center (Poland); MIUR project (Italy)
[20108T4XTM]; Thalis program - EU-ESF; Greek NSRF; Aristeia program -
EU-ESF; Qatar National Research Fund; Rachadapisek Sompot Fund for
Postdoctoral Fellowship, Chulalongkorn University (Thailand);
Chulalongkorn Academic into Its 2nd Century Project Advancement Project
(Thailand); Welch Foundation [C-1845]; Ministry of Science and
Technology
FX We congratulate our colleagues in the CERN accelerator departments for
the excellent performance of the LHC and thank the technical and
administrative staffs at CERN and at other CMS institutes for their
contributions to the success of the CMS effort. In addition, we
gratefully acknowledge the computing centers and personnel of the
Worldwide LHC Computing Grid for delivering so effectively the computing
infrastructure essential to our analyses.; Finally, we acknowledge the
enduring support for the construction and operation of the LHC and the
CMS detector provided by the following funding agencies: the Austrian
Federal Ministry of Science, Research and Economy and the Austrian
Science Fund; the Belgian Fonds de la Recherche Scientifique, and Fonds
voor Wetenschappelijk Onderzoek; the Brazilian Funding Agencies (CNPq,
CAPES, FAPERJ, and FAPESP); the Bulgarian Ministry of Education and
Science; CERN; the Chinese Academy of Sciences, Ministry of Science and
Technology, and National Natural Science Foundation of China; the
Colombian Funding Agency (COLCIENCIAS); the Croatian Ministry of
Science, Education and Sport, and the Croatian Science Foundation; the
Research Promotion Foundation, Cyprus; the Ministry of Education and
Research, Estonian Research Council via IUT23-4 and IUT23-6 and European
Regional Development Fund, Estonia; the Academy of Finland, Finnish
Ministry of Education and Culture, and Helsinki Institute of Physics;
the Institut National de Physique Nucleaire et de Physique des
Particules / CNRS, and Commissariat a l'Energie Atomique et aux Energies
Alternatives / CEA, France; the Bundesministerium fur Bildung und
Forschung, Deutsche Forschungsgemeinschaft, and Helmholtz-Gemeinschaft
Deutscher Forschungszentren, Germany; the General Secretariat for
Research and Technology, Greece; the National Scientific Research
Foundation, and National Innovation Office, Hungary; the Department of
Atomic Energy and the Department of Science and Technology, India; the
Institute for Studies in Theoretical Physics and Mathematics, Iran; the
Science Foundation, Ireland; the Istituto Nazionale di Fisica Nucleare,
Italy; the Ministry of Science, ICT and Future Planning, and National
Research Foundation (NRF), Republic of Korea; the Lithuanian Academy of
Sciences; the Ministry of Education, and University of Malaya
(Malaysia); the Mexican Funding Agencies (BUAP, CINVESTAV, CONACYT, LNS,
SEP, and UASLP-FAI); the Ministry of Business, Innovation and
Employment, New Zealand; the Pakistan Atomic Energy Commission; the
Ministry of Science and Higher Education and the National Science
Center, Poland; the Fundacao para a Ciencia e a Tecnologia, Portugal;
JINR, Dubna; the Ministry of Education and Science of the Russian
Federation, the Federal Agency of Atomic Energy of the Russian
Federation, Russian Academy of Sciences, and the Russian Foundation for
Basic Research; the Ministry of Education, Science and Technological
Development of Serbia; the Secretaria de Estado de Investigacion,
Desarrollo e Innovacion and Programa Consolider-Ingenio 2010, Spain; the
Swiss Funding Agencies (ETH Board, ETH Zurich, PSI, SNF, UniZH, Canton
Zurich, and SER); the Ministry of Science and Technology, Taipei; the
Thailand Center of Excellence in Physics, the Institute for the
Promotion of Teaching Science and Technology of Thailand, Special Task
Force for Activating Research and the National Science and Technology
Development Agency of Thailand; the Scientific and Technical Research
Council of Turkey, and Turkish Atomic Energy Authority; the National
Academy of Sciences of Ukraine, and State Fund for Fundamental
Researches, Ukraine; the Science and Technology Facilities Council, UK;
the US Department of Energy, and the US National Science Foundation.
Individuals have received support from the Marie-Curie program and the
European Research Council and EPLANET (European Union); the Leventis
Foundation; the A. P.; Sloan Foundation; the Alexander von Humboldt
Foundation; the Belgian Federal Science Policy Office; the Fonds pour la
Formation a la Recherche dans l'Industrie et dans l'Agriculture
(FRIA-Belgium); the Agentschap voor Innovatie door Wetenschap en
Technologie (IWT-Belgium); the Ministry of Education, Youth and Sports
(MEYS) of the Czech Republic; the Council of Science and Industrial
Research, India; the HOMING PLUS program of the Foundation for Polish
Science, cofinanced from European Union, Regional Development Fund; the
Mobility Plus program of the Ministry of Science and Higher Education
(Poland); the OPUS program of the National Science Center (Poland); MIUR
project 20108T4XTM (Italy); the Thalis and Aristeia programs cofinanced
by EU-ESF and the Greek NSRF; the National Priorities Research Program
by Qatar National Research Fund; the Rachadapisek Sompot Fund for
Postdoctoral Fellowship, Chulalongkorn University (Thailand); the
Chulalongkorn Academic into Its 2nd Century Project Advancement Project
(Thailand); and the Welch Foundation, Contract No. C-1845.
NR 56
TC 0
Z9 0
U1 22
U2 22
PU AMER PHYSICAL SOC
PI COLLEGE PK
PA ONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA
SN 2470-0010
EI 2470-0029
J9 PHYS REV D
JI Phys. Rev. D
PD OCT 12
PY 2016
VL 94
IS 7
AR 072002
DI 10.1103/PhysRevD.94.072002
PG 25
WC Astronomy & Astrophysics; Physics, Particles & Fields
SC Astronomy & Astrophysics; Physics
GA DZ1WN
UT WOS:000385632500001
ER
PT J
AU Lyubimov, AY
Uervirojnangkoorn, M
Zeldin, OB
Zhou, QJ
Zhao, MG
Brewster, AS
Michels-Clark, T
Holton, JM
Sauter, NK
Weis, WI
Brunger, AT
AF Lyubimov, Artem Y.
Uervirojnangkoorn, Monarin
Zeldin, Oliver B.
Zhou, Qiangjun
Zhao, Minglei
Brewster, Aaron S.
Michels-Clark, Tara
Holton, James M.
Sauter, Nicholas K.
Weis, William I.
Brunger, Axel T.
TI Advances in X-ray free electron laser (XFEL) diffraction data processing
applied to the crystal structure of the synaptotagmin-1 / SNARE complex
SO ELIFE
LA English
DT Article
ID FEMTOSECOND CRYSTALLOGRAPHY; DATA-COLLECTION; DATA QUALITY; REFINEMENT;
MICROCRYSTALS; SYSTEM; PARTIALITY; GEOMETRY; MODEL
AB X-ray free electron lasers (XFELs) reduce the effects of radiation damage on macromolecular diffraction data and thereby extend the limiting resolution. Previously, we adapted classical post-refinement techniques to XFEL diffraction data to produce accurate diffraction data sets from a limited number of diffraction images (Uervirojnangkoorn et al., 2015), and went on to use these techniques to obtain a complete data set from crystals of the synaptotagmin-1 / SNARE complex and to determine the structure at 3.5 angstrom resolution (Zhou et al., 2015). Here, we describe new advances in our methods and present a reprocessed XFEL data set of the synaptotagmin-1 / SNARE complex. The reprocessing produced small improvements in electron density maps and the refined atomic model. The maps also contained more information than those of a lower resolution (4.1 angstrom) synchrotron data set. Processing a set of simulated XFEL diffraction images revealed that our methods yield accurate data and atomic models.
C1 [Lyubimov, Artem Y.; Uervirojnangkoorn, Monarin; Zeldin, Oliver B.; Zhou, Qiangjun; Zhao, Minglei; Weis, William I.; Brunger, Axel T.] Stanford Univ, Dept Mol & Cellular Physiol, Stanford, CA 94305 USA.
[Lyubimov, Artem Y.; Uervirojnangkoorn, Monarin; Zeldin, Oliver B.; Zhou, Qiangjun; Zhao, Minglei; Brunger, Axel T.] Stanford Univ, Neurol & Neurol Sci, Stanford, CA 94305 USA.
[Lyubimov, Artem Y.; Uervirojnangkoorn, Monarin; Zeldin, Oliver B.; Zhou, Qiangjun; Zhao, Minglei; Weis, William I.; Brunger, Axel T.] Stanford Univ, Struct Biol, Stanford, CA 94305 USA.
[Lyubimov, Artem Y.; Uervirojnangkoorn, Monarin; Zeldin, Oliver B.; Zhou, Qiangjun; Zhao, Minglei; Weis, William I.; Brunger, Axel T.] Stanford Univ, Photon Sci, Stanford, CA 94305 USA.
[Lyubimov, Artem Y.; Uervirojnangkoorn, Monarin; Zeldin, Oliver B.; Zhou, Qiangjun; Zhao, Minglei; Brunger, Axel T.] Stanford Univ, Howard Hughes Med Inst, Stanford, CA 94305 USA.
[Brewster, Aaron S.; Michels-Clark, Tara; Holton, James M.; Sauter, Nicholas K.] Lawrence Berkeley Natl Lab, Mol Biophys & Integrated Bioimaging Div, Berkeley, CA USA.
[Holton, James M.] SKAC Natl Accelerator Lab, Stanford Synchrotron Radiat Lightsource, Menlo Pk, CA USA.
[Holton, James M.] Univ Calif San Francisco, Dept Biochem & Biophys, San Francisco, CA 94143 USA.
RP Weis, WI; Brunger, AT (reprint author), Stanford Univ, Dept Mol & Cellular Physiol, Stanford, CA 94305 USA.; Brunger, AT (reprint author), Stanford Univ, Neurol & Neurol Sci, Stanford, CA 94305 USA.; Weis, WI; Brunger, AT (reprint author), Stanford Univ, Struct Biol, Stanford, CA 94305 USA.; Weis, WI; Brunger, AT (reprint author), Stanford Univ, Photon Sci, Stanford, CA 94305 USA.; Brunger, AT (reprint author), Stanford Univ, Howard Hughes Med Inst, Stanford, CA 94305 USA.
EM bill.weis@stanford.edu; brunger@stanford.edu
FU Howard Hughes Medical Institute Collaborative Innovation Award; National
Institutes of Health [R01GM102520, R01GM117126, P41 GM103403, S10
RR029205]
FX Howard Hughes Medical Institute Collaborative Innovation Award William I
Weis Axel T Brunger; National Institutes of Health R01GM102520 Nicholas
K Sauter; National Institutes of Health R01GM117126 Nicholas K Sauter;
National Institute of General Medical Sciences P41 GM103403 Axel T
Brunger; National Institutes of Health S10 RR029205 Axel T Brunger; The
funders had no role in study design, data collection and interpretation,
or the decision to submit the work for publication.
NR 41
TC 2
Z9 2
U1 2
U2 2
PU ELIFE SCIENCES PUBLICATIONS LTD
PI CAMBRIDGE
PA SHERATON HOUSE, CASTLE PARK, CAMBRIDGE, CB3 0AX, ENGLAND
SN 2050-084X
J9 ELIFE
JI eLife
PD OCT 12
PY 2016
VL 5
AR e18740
DI 10.7554/eLife.18740
PG 18
WC Biology
SC Life Sciences & Biomedicine - Other Topics
GA EC1NW
UT WOS:000387873700001
ER
PT J
AU Kim, H
Kim, H
Ding, Z
Lee, MH
Lim, K
Yoon, G
Kang, K
AF Kim, Hyungsub
Kim, Haegyeom
Ding, Zhang
Lee, Myeong Hwan
Lim, Kyungmi
Yoon, Gabin
Kang, Kisuk
TI Recent Progress in Electrode Materials for Sodium-Ion Batteries
SO ADVANCED ENERGY MATERIALS
LA English
DT Review
ID HIGH-PERFORMANCE ANODE; X-RAY-DIFFRACTION; LONG-CYCLE-LIFE; RECHARGEABLE
LITHIUM BATTERIES; ELECTRICAL ENERGY-STORAGE; HIGH-CAPACITY CATHODE;
IMPROVED ELECTROCHEMICAL PERFORMANCE; GRAPHITE-INTERCALATION COMPOUNDS;
SINGLE-CRYSTALLINE NA0.44MNO2; CARBON-COATED NA3V2(PO4)(3)
AB Grid-scale energy storage systems (ESSs) that can connect to sustainable energy resources have received great attention in an effort to satisfy ever-growing energy demands. Although recent advances in Li-ion battery (LIB) technology have increased the energy density to a level applicable to grid-scale ESSs, the high cost of Li and transition metals have led to a search for lower-cost battery system alternatives. Based on the abundance and accessibility of Na and its similar electrochemistry to the well-established LIB technology, Na-ion batteries (NIBs) have attracted significant attention as an ideal candidate for grid-scale ESSs. Since research on NIB chemistry resurged in 2010, various positive and negative electrode materials have been synthesized and evaluated for NIBs. Nonetheless, studies on NIB chemistry are still in their infancy compared with LIB technology, and further improvements are required in terms of energy, power density, and electrochemical stability for commercialization. Most recent progress on electrode materials for NIBs, including the discovery of new electrode materials and their Na storage mechanisms, is briefly reviewed. In addition, efforts to enhance the electrochemical properties of NIB electrode materials as well as the challenges and perspectives involving these materials are discussed.
C1 [Kim, Hyungsub; Kim, Haegyeom; Ding, Zhang; Lee, Myeong Hwan; Lim, Kyungmi; Yoon, Gabin; Kang, Kisuk] Seoul Natl Univ, Res Inst Adv Mat, Dept Mat Sci & Engn, Seoul 08826, South Korea.
[Kim, Hyungsub; Yoon, Gabin; Kang, Kisuk] Seoul Natl Univ, Ctr Nanoparticle Res, IBS, Seoul 08826, South Korea.
[Kim, Haegyeom] Lawrence Berkeley Natl Lab, 1 Cyclotron Rd, Berkeley, CA 94720 USA.
[Ding, Zhang] Taiyuan Univ Technol, Coll Chem & Chem Engn, Taiyuan 030024, Shanxi, Peoples R China.
RP Kang, K (reprint author), Seoul Natl Univ, Res Inst Adv Mat, Dept Mat Sci & Engn, Seoul 08826, South Korea.; Kang, K (reprint author), Seoul Natl Univ, Ctr Nanoparticle Res, IBS, Seoul 08826, South Korea.
EM matlgen1@snu.ac.kr
FU Energy Efficiency & Resources of the Korea Institute of Energy
Technology Evaluation and Planning (KETEP) - Korea government Ministry
of Trade, Industry Energy (MOTIE) [20132020000270]; [IBS-R006-G1]
FX This work was supported by (i) Project Code. (IBS-R006-G1) and (ii)
Energy Efficiency & Resources of the Korea Institute of Energy
Technology Evaluation and Planning (KETEP) grant funded by the Korea
government Ministry of Trade, Industry & Energy (MOTIE) (No.
20132020000270). H.K. and H.K. contributed equally to this paper.
NR 470
TC 5
Z9 5
U1 476
U2 476
PU WILEY-V C H VERLAG GMBH
PI WEINHEIM
PA POSTFACH 101161, 69451 WEINHEIM, GERMANY
SN 1614-6832
EI 1614-6840
J9 ADV ENERGY MATER
JI Adv. Energy Mater.
PD OCT 12
PY 2016
VL 6
IS 19
AR 1600943
DI 10.1002/aenm.201600943
PG 38
WC Chemistry, Physical; Energy & Fuels; Materials Science,
Multidisciplinary; Physics, Applied; Physics, Condensed Matter
SC Chemistry; Energy & Fuels; Materials Science; Physics
GA EB1SK
UT WOS:000387134800011
ER
PT J
AU Tang, JY
Yuan, P
Cai, CL
Fu, YB
Ma, XH
AF Tang, Jiayong
Yuan, Ping
Cai, Chuanlin
Fu, Yanbao
Ma, Xiaohua
TI Combining Nature-Inspired, Graphene-Wrapped Flexible Electrodes with
Nanocomposite Polymer Electrolyte for Asymmetric Capacitive Energy
Storage
SO ADVANCED ENERGY MATERIALS
LA English
DT Article
ID SUPERCAPACITOR APPLICATIONS; FACILE SYNTHESIS; FILM ELECTRODES; ANODE
MATERIALS; LITHIUM-ION; PERFORMANCE; NANOPARTICLES; FABRICATION;
COMPOSITES; DESIGN
AB Two kinds of free-standing electrodes, reduced graphene oxide (rGO)-wrapped Fe-doped MnO2 composite (G-MFO) and rGO-wrapped hierarchical porous carbon microspheres composite (G-HPC) are fabricated using a frozen lake-inspired, bubble-assistance method. This configuration fully enables utilization of the synergistic effects from both components, endowing the materials to be excellent electrodes for flexible and lightweight electrochemical capacitors. Moreover, a nonaqueous HPC-doped gel polymer electrolyte (GPE-HPC) is employed to broad voltage window and improve heat resistance. A fabricated asymmetric supercapacitor based on G-MFO cathode and G-HPC anode with GPE-HPC electrolyte achieves superior flexibility and reliability, enhanced energy/power density, and outstanding cycling stability. The ability to power light-emitting diodes also indicates the feasibility for practical use. Therefore, it is believed that this novel design may hold great promise for future flexible electronic devices.
C1 [Tang, Jiayong; Yuan, Ping; Cai, Chuanlin; Ma, Xiaohua] Fudan Univ, Dept Mat Sci, Shanghai 200433, Peoples R China.
[Fu, Yanbao] Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Environm & Energy Technol Div, Berkeley, CA 94720 USA.
RP Ma, XH (reprint author), Fudan Univ, Dept Mat Sci, Shanghai 200433, Peoples R China.
EM xhma@fudan.edu.cn
FU State Key 973 Program of PRC [2011CB605704]; National Natural Science
Foundation of China [U1201241, 51372041, 51202034, 51201035]
FX J.T. and P.Y. contributed equally to this work. This work was
financially supported by the State Key 973 Program of PRC (Grant No.
2011CB605704) and the National Natural Science Foundation of China
(Grants No. U1201241, 51372041, 51202034, and 51201035).
NR 45
TC 1
Z9 1
U1 83
U2 83
PU WILEY-V C H VERLAG GMBH
PI WEINHEIM
PA POSTFACH 101161, 69451 WEINHEIM, GERMANY
SN 1614-6832
EI 1614-6840
J9 ADV ENERGY MATER
JI Adv. Energy Mater.
PD OCT 12
PY 2016
VL 6
IS 19
AR 1600813
DI 10.1002/aenm.201600813
PG 11
WC Chemistry, Physical; Energy & Fuels; Materials Science,
Multidisciplinary; Physics, Applied; Physics, Condensed Matter
SC Chemistry; Energy & Fuels; Materials Science; Physics
GA EB1SK
UT WOS:000387134800009
ER
PT J
AU Weng, W
Huang, JH
Shkrob, IA
Zhang, L
Zhang, ZC
AF Weng, Wei
Huang, Jinhua
Shkrob, Ilya A.
Zhang, Lu
Zhang, Zhengcheng
TI Redox Shuttles with Axisymmetric Scaffold for Overcharge Protection of
Lithium-Ion Batteries
SO ADVANCED ENERGY MATERIALS
LA English
DT Article
ID HIGH-ENERGY CATHODE; NONAQUEOUS ELECTROLYTES; FLOW BATTERY; CELLS;
STABILITY; ADDITIVES; DENSITY
AB The derivatives of 1,4-dimethoxybenzene are thus far the best performing redox shuttle additives for overcharge protection of Li-ion batteries. The most durable molecules of this kind typically possess two in-plane methoxy groups that are equivalent by inversion symmetry. However, such geometry leads to a vanishing average dipole moment that causes poor solubility of these molecules in carbonate-based electrolytes. In this study, a novel redox shuttle additive, 1,2,3,4-tetrahydro-6,7-dimethoxy-1,1,4,4-tetramethyl-naphthalene (TDTN), is introduced. It has been demonstrated that reversible oxidation at 4.05 V versus Li+/Li, high polarity, high solubility (around 0.4 M), and excellent electrochemical stability (150 overcharge cycles at C/2 rate with 100% overcharge) can all be achieved simultaneously by the imposition of axial symmetry in the corresponding radical cation that is generated by electrochemical oxidation of TDTN in the battery. The intricate interplay between the symmetry and the chemical stability of the radical cation is scrutinized using magnetic resonance spectroscopy and electron structure modeling.
C1 [Weng, Wei; Huang, Jinhua; Shkrob, Ilya A.; Zhang, Lu; Zhang, Zhengcheng] Argonne Natl Lab, Chem Sci & Engn Div, 9700 S Cass Ave, Argonne, IL 60439 USA.
[Huang, Jinhua; Shkrob, Ilya A.; Zhang, Lu; Zhang, Zhengcheng] Argonne Natl Lab, Joint Ctr Energy Storage Res, 9700 S Cass Ave, Argonne, IL 60439 USA.
RP Zhang, ZC (reprint author), Argonne Natl Lab, Chem Sci & Engn Div, 9700 S Cass Ave, Argonne, IL 60439 USA.; Zhang, ZC (reprint author), Argonne Natl Lab, Joint Ctr Energy Storage Res, 9700 S Cass Ave, Argonne, IL 60439 USA.
EM zzhang@anl.gov
FU Center for Electrical Energy Storage: Tailored Interfaces, an Energy
Frontier Research Center - U.S. Department of Energy, Office of Science,
Office of Basic Energy Sciences; Joint Center for Energy Storage
Research (JCESR), an energy innovation hub - U.S. Department of Energy,
Office of Science, Basic Energy Sciences; U.S. Department of Energy
[DE-ACOZ-06CH11357]
FX This work was supported by the Center for Electrical Energy Storage:
Tailored Interfaces, an Energy Frontier Research Center funded by the
U.S. Department of Energy, Office of Science, Office of Basic Energy
Sciences. This work was also supported as part of the Joint Center for
Energy Storage Research (JCESR), an energy innovation hub funded by the
U.S. Department of Energy, Office of Science, Basic Energy Sciences.
Argonne National Laboratory is operated for the U.S. Department of
Energy by UChicago Argonne, LLC, under contract DE-ACOZ-06CH11357.
NR 31
TC 0
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U1 17
U2 17
PU WILEY-V C H VERLAG GMBH
PI WEINHEIM
PA POSTFACH 101161, 69451 WEINHEIM, GERMANY
SN 1614-6832
EI 1614-6840
J9 ADV ENERGY MATER
JI Adv. Energy Mater.
PD OCT 12
PY 2016
VL 6
IS 19
AR 1600795
DI 10.1002/aenm.201600795
PG 7
WC Chemistry, Physical; Energy & Fuels; Materials Science,
Multidisciplinary; Physics, Applied; Physics, Condensed Matter
SC Chemistry; Energy & Fuels; Materials Science; Physics
GA EB1SK
UT WOS:000387134800008
ER
PT J
AU Schulze-Gahmen, U
Echeverria, I
Stjepanovic, G
Bai, Y
Lu, HS
Schneidman-Duhovny, D
Doudna, JA
Zhou, Q
Sali, A
Hurley, JH
AF Schulze-Gahmen, Ursula
Echeverria, Ignacia
Stjepanovic, Goran
Bai, Yun
Lu, Huasong
Schneidman-Duhovny, Dina
Doudna, Jennifer A.
Zhou, Qiang
Sali, Andrej
Hurley, James H.
TI Insights into HIV-1 proviral transcription from integrative structure
and dynamics of the Tat:AFF4:P-TEFb:TAR complex
SO ELIFE
LA English
DT Article
ID RNA-POLYMERASE-II; TAR RNA; ELONGATION COMPLEX; CRYSTAL-STRUCTURE;
CYCLIN T1; STRUCTURE REFINEMENT; MASS-SPECTROMETRY; HIGH-AFFINITY;
PROTEIN; RECOGNITION
AB HIV-1 Tat hijacks the human superelongation complex (SEC) to promote proviral transcription. Here we report the 5.9 angstrom structure of HIV-1 TAR in complex with HIV-1 Tat and human AFF4, CDK9, and CycT1. The TAR central loop contacts the CycT1 Tat-TAR recognition motif (TRM) and the second Tat Zn2+-binding loop. Hydrogen-deuterium exchange (HDX) shows that AFF4 helix 2 is stabilized in the TAR complex despite not touching the RNA, explaining how it enhances TAR binding to the SEC 50-fold. RNA SHAPE and SAXS data were used to help model the extended (Tat Arginine-Rich Motif) ARM, which enters the TAR major groove between the bulge and the central loop. The structure and functional assays collectively support an integrative structure and a bipartite binding model, wherein the TAR central loop engages the CycT1 TRM and compact core of Tat, while the TAR major groove interacts with the extended Tat ARM.
C1 [Schulze-Gahmen, Ursula; Stjepanovic, Goran; Bai, Yun; Lu, Huasong; Doudna, Jennifer A.; Zhou, Qiang; Hurley, James H.] Univ Calif Berkeley, Dept Mol & Cell Biol, 229 Stanley Hall, Berkeley, CA 94720 USA.
[Schulze-Gahmen, Ursula; Stjepanovic, Goran; Bai, Yun; Lu, Huasong; Doudna, Jennifer A.; Zhou, Qiang; Hurley, James H.] Univ Calif Berkeley, Calif Inst Quantitat Biosci, Berkeley, CA 94720 USA.
[Echeverria, Ignacia; Schneidman-Duhovny, Dina; Sali, Andrej] Univ Calif San Francisco, Dept Bioengn & Therapeut Sci, San Francisco, CA 94143 USA.
[Echeverria, Ignacia; Schneidman-Duhovny, Dina; Sali, Andrej] Univ Calif San Francisco, Dept Pharmaceut Chem, San Francisco, CA 94143 USA.
[Echeverria, Ignacia; Schneidman-Duhovny, Dina; Sali, Andrej] Univ Calif San Francisco, Calif Inst Quantitat Biosci, San Francisco, CA 94143 USA.
[Stjepanovic, Goran; Doudna, Jennifer A.; Hurley, James H.] Lawrence Berkeley Natl Lab, Mol Biophys & Integrated Bioimaging Div, Berkeley, CA USA.
[Doudna, Jennifer A.] Univ Calif Berkeley, Howard Hughes Med Inst, Berkeley, CA 94720 USA.
[Doudna, Jennifer A.] Univ Calif Berkeley, Dept Chem, Berkeley, CA 94720 USA.
RP Hurley, JH (reprint author), Univ Calif Berkeley, Dept Mol & Cell Biol, 229 Stanley Hall, Berkeley, CA 94720 USA.; Hurley, JH (reprint author), Univ Calif Berkeley, Calif Inst Quantitat Biosci, Berkeley, CA 94720 USA.; Hurley, JH (reprint author), Lawrence Berkeley Natl Lab, Mol Biophys & Integrated Bioimaging Div, Berkeley, CA USA.
EM jimhurley@berkeley.edu
FU National Institutes of Health [P50GM082250]; National Institute of
Allergy and Infectious Diseases [R01AI041757, R01AI095057]
FX National Institutes of Health P50GM082250 Jennifer A Doudna Andrej Sali
James H Hurley; National Institute of Allergy and Infectious Diseases
R01AI041757 Qiang Zhou; National Institute of Allergy and Infectious
Diseases R01AI095057 Qiang Zhou
NR 66
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Z9 0
U1 5
U2 5
PU ELIFE SCIENCES PUBLICATIONS LTD
PI CAMBRIDGE
PA SHERATON HOUSE, CASTLE PARK, CAMBRIDGE, CB3 0AX, ENGLAND
SN 2050-084X
J9 ELIFE
JI eLife
PD OCT 12
PY 2016
VL 5
AR e15910
DI 10.7554/eLife.15910
PG 21
WC Biology
SC Life Sciences & Biomedicine - Other Topics
GA EA5QQ
UT WOS:000386677300001
ER
PT J
AU Kibria, MG
Qiao, RM
Yang, WL
Boukahil, I
Kong, XH
Chowdhury, FA
Trudeau, ML
Ji, W
Guo, H
Himpsel, FJ
Vayssieres, L
Mi, ZT
AF Kibria, Md Golam
Qiao, Ruimin
Yang, Wanli
Boukahil, Idris
Kong, Xianghua
Chowdhury, Faqrul Alam
Trudeau, Michel L.
Ji, Wei
Guo, Hong
Himpsel, F. J.
Vayssieres, Lionel
Mi, Zetian
TI Atomic-Scale Origin of Long-Term Stability and High Performance of p-GaN
Nanowire Arrays for Photocatalytic Overall Pure Water Splitting
SO ADVANCED MATERIALS
LA English
DT Article
DE artificial photosynthesis; metal nitride; N-terminated surfaces;
polarization dependence; wurtzite structure; X-ray spectroscopy
ID X-RAY-ABSORPTION; MOLECULAR-BEAM EPITAXY; GROUP-III NITRIDES; N-TYPE
GAN; TO-HYDROGEN CONVERSION; PHOTOELECTROCHEMICAL PROPERTIES; ARTIFICIAL
PHOTOSYNTHESIS; GROWTH; PHOTOANODE; OXIDATION
AB The atomic-scale origin of the unusually high performance and long-term stability of wurtzite p-GaN oriented nanowire arraysis revealed. Nitrogen termination of both the polar (000 (1) over bar) top face and the non polar (10 (1) over bar0) side faces of the nanowires is essential for long-term stability and high efficiency. Such a distinct atomic configuration ensures not only stability against (photo) oxidation in air and in water/electrolyte but, as importantly, also provides the necessary overall reverse crystal polarization needed for efficient hole extraction in p-GaN.
C1 [Kibria, Md Golam; Chowdhury, Faqrul Alam; Mi, Zetian] McGill Univ, Dept Elect & Comp Engn, Montreal, PQ H3A 0E9, Canada.
[Qiao, Ruimin; Yang, Wanli] Lawrence Berkeley Natl Lab, Adv Light Source, Berkeley, CA 94720 USA.
[Boukahil, Idris; Himpsel, F. J.] Univ Wisconsin, Dept Phys, 1150 Univ Ave, Madison, WI 53706 USA.
[Kong, Xianghua; Guo, Hong] McGill Univ, Dept Phys, 3600 Univ St, Montreal, PQ H3A 2T8, Canada.
[Kong, Xianghua; Ji, Wei] Renmin Univ China, Dept Phys, Beijing 100872, Peoples R China.
[Kong, Xianghua; Ji, Wei] Renmin Univ China, Beijing Key Lab Optoelect Funct Mat & Micronano D, Beijing 100872, Peoples R China.
[Trudeau, Michel L.] Hydro Quebec, IREQ, Sci Mat, Varennes, PQ J3X 1S1, Canada.
[Vayssieres, Lionel] Xi An Jiao Tong Univ, Sch Energy & Power Engn, Int Res Ctr Renewable Energy, Xian 710049, Peoples R China.
RP Mi, ZT (reprint author), McGill Univ, Dept Elect & Comp Engn, Montreal, PQ H3A 0E9, Canada.; Himpsel, FJ (reprint author), Univ Wisconsin, Dept Phys, 1150 Univ Ave, Madison, WI 53706 USA.; Vayssieres, L (reprint author), Xi An Jiao Tong Univ, Sch Energy & Power Engn, Int Res Ctr Renewable Energy, Xian 710049, Peoples R China.
EM fhimpsel@wisc.edu; lionelv@xjtu.edu.cn; zetian.mi@mcgill.ca
RI Yang, Wanli/D-7183-2011; Ji, Wei/G-6097-2010; Qiao, Ruimin/E-9023-2013
OI Yang, Wanli/0000-0003-0666-8063; Ji, Wei/0000-0001-5249-6624;
FU U.S. Department of Energy, Office of Basic Energy Sciences
[DE-AC02-05CH11231, DE-SC0006931]; Natural Sciences and Engineering
Research Council of Canada (NSERC); Climate Change and Emissions
Management (CCEMC) Corporation; International Research Center for
Renewable Energy, Xi'an Jiaotong University; Thousand Talents plan;
National Natural Science Foundation of China [51202186]; Natural
Sciences and Engineering Research Council of Canada; Chinese Scholarship
Council
FX F.J.H., L.V., and Z.M. contributed equally to this work. L.V. proposed
and managed the entire project with Z.M. and F.J.H. M.G.K., and F.A.C.
prepared the samples. R.Q., F.J.H., and W.Y. managed the beamline
experiments and the experimental setup. R.Q. and F.J.H. performed the
synchrotron experiments and I.B. the data analysis. X.K., W.J., and H.G.
managed and performed the DFT study. M.L.T. managed and performed the
STEM, EELS, and HAADF studies. All the authors actively discussed the
results and commented on the manuscript. This research was supported by
the U.S. Department of Energy, Office of Basic Energy Sciences under the
Contracts DE-AC02-05CH11231 (ALS), DE-SC0006931 (end station), by the
Natural Sciences and Engineering Research Council of Canada (NSERC) and
the Climate Change and Emissions Management (CCEMC) Corporation, by the
International Research Center for Renewable Energy, Xi'an Jiaotong
University, the Thousand Talents plan and the National Natural Science
Foundation of China (No. 51202186), and by the Natural Sciences and
Engineering Research Council of Canada. R.Q. thanks the LDRD program at
Lawrence Berkeley National Laboratory. X.K. wishes to thank the Chinese
Scholarship Council for the support. The authors wish to thank
CalcuQuebec and Compute Canada for offering their computation
facilities. The authors also wish to thank Dr. S. Zhao and Dr. Q. Wang
for their help with the MBE growth and micro-Raman measurement,
respectively.
NR 70
TC 1
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U1 57
U2 57
PU WILEY-V C H VERLAG GMBH
PI WEINHEIM
PA POSTFACH 101161, 69451 WEINHEIM, GERMANY
SN 0935-9648
EI 1521-4095
J9 ADV MATER
JI Adv. Mater.
PD OCT 12
PY 2016
VL 28
IS 38
BP 8388
EP 8397
DI 10.1002/adma.201602274
PG 10
WC Chemistry, Multidisciplinary; Chemistry, Physical; Nanoscience &
Nanotechnology; Materials Science, Multidisciplinary; Physics, Applied;
Physics, Condensed Matter
SC Chemistry; Science & Technology - Other Topics; Materials Science;
Physics
GA DZ8EM
UT WOS:000386103700006
PM 27456856
ER
PT J
AU Naughton, KL
Phan, L
Leung, EM
Kautz, R
Lin, QY
Van Dyke, Y
Marmiroli, B
Sartori, B
Arvai, A
Li, S
Pique, ME
Naeim, M
Kerr, JP
Aquino, MJ
Roberts, VA
Getzoff, ED
Zhu, CH
Bernstorff, S
Gorodetsky, AA
AF Naughton, Kyle L.
Phan, Long
Leung, Erica M.
Kautz, Rylan
Lin, Qiyin
Van Dyke, Yegor
Marmiroli, Benedetta
Sartori, Barbara
Arvai, Andy
Li, Sheng
Pique, Michael E.
Naeim, Mahan
Kerr, Justin P.
Aquino, Mercedeez J.
Roberts, Victoria A.
Getzoff, Elizabeth D.
Zhu, Chenhui
Bernstorff, Sigrid
Gorodetsky, Alon A.
TI Self-Assembly of the Cephalopod Protein Reflectin
SO ADVANCED MATERIALS
LA English
DT Article
DE cephalopods; functional coatings; proteins; self-assembly; X-ray
scattering
ID SMALL-ANGLE SCATTERING; X-RAY-SCATTERING; EXCHANGE-MASS-SPECTROMETRY;
CASEIN MICELLES; BIOLOGICAL MACROMOLECULES; NEUTRON-SCATTERING; SQUID;
HYDROGEN/DEUTERIUM; BIOPHOTONICS; IRIDESCENCE
AB Films from the cephalopod protein reflectin demonstrate multifaceted functionality as infrared camouflage coatings, proton transport media, and substrates for growth of neural stem cells. A detailed study of the in vitro formation, structural characteristics, and stimulus response of such films is presented. The reported observations hold implications for the design and development of advanced cephalopod-inspired functional materials.
C1 [Naughton, Kyle L.] Univ Calif Irvine, Dept Phys & Astron, Irvine, CA 92697 USA.
[Phan, Long; Leung, Erica M.; Kautz, Rylan; Van Dyke, Yegor; Naeim, Mahan; Kerr, Justin P.; Aquino, Mercedeez J.; Gorodetsky, Alon A.] Univ Calif Irvine, Dept Chem Engn & Mat Sci, Irvine, CA 92697 USA.
[Lin, Qiyin] Univ Calif Irvine, Lab Electron & Xray Instrumentat, Irvine, CA 92697 USA.
[Marmiroli, Benedetta; Sartori, Barbara] Graz Univ Technol, Inst Inorgan Chem, Stremayrgasse 9-4, A-8010 Graz, Austria.
[Arvai, Andy; Pique, Michael E.; Getzoff, Elizabeth D.] Scripps Res Inst, Dept Integrat Struct & Computat Biol, La Jolla, CA 92037 USA.
[Li, Sheng] Univ Calif San Diego, Dept Med, San Diego, CA 92093 USA.
[Roberts, Victoria A.] Univ Calif San Diego, San Diego Supercomp Ctr, La Jolla, CA 92093 USA.
[Getzoff, Elizabeth D.] Scripps Res Inst, Skaggs Inst Chem Biol, La Jolla, CA 92037 USA.
[Zhu, Chenhui] Lawrence Berkeley Natl Lab, Adv Light Source, Berkeley, CA 94720 USA.
[Bernstorff, Sigrid] Elettra Sincrotrone Trieste, Str Statale 14,Km 163-5, I-34149 Trieste, Italy.
[Gorodetsky, Alon A.] Univ Calif Irvine, Dept Chem, Irvine, CA 92697 USA.
RP Gorodetsky, AA (reprint author), Univ Calif Irvine, Dept Chem Engn & Mat Sci, Irvine, CA 92697 USA.; Gorodetsky, AA (reprint author), Univ Calif Irvine, Dept Chem, Irvine, CA 92697 USA.
EM alon.gorodetsky@uci.edu
FU Air Force Office of Scientific Research [FA9550-14-1-0144]; Office of
Science, Office of Basic Energy Sciences, of the Department of Energy
[DE-AC02-05CH11231]; Office of Science [DE-AC02-06CH11357]; National
Science Foundation Center for Chemistry at the Space-Time Limit
[CHE-082913]
FX The authors thank Chiharu Hitomi for help with preparing the DXMS
samples. The authors are grateful to the Air Force Office of Scientific
Research (FA9550-14-1-0144) for its financial support. The authors
acknowledge the use of beamline 7.3.3 at the Advanced Light Source,
which was supported by the Director of the Office of Science, Office of
Basic Energy Sciences, of the Department of Energy under Contract No.
DE-AC02-05CH11231. The authors also acknowledge the use of beamline
5-ID-D at the Advanced Photon Source, a U.S. Department of Energy Office
of Science User Facility operated for the Office of Science by Argonne
National Laboratory under Contract No. DE-AC02-06CH11357. Finally, the
authors acknowledge the use of SEM instrumentation at the UC Irvine
Materials Research Institute (IMRI), which was funded in part by the
National Science Foundation Center for Chemistry at the Space-Time Limit
(CHE-082913).
NR 81
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Z9 0
U1 37
U2 37
PU WILEY-V C H VERLAG GMBH
PI WEINHEIM
PA POSTFACH 101161, 69451 WEINHEIM, GERMANY
SN 0935-9648
EI 1521-4095
J9 ADV MATER
JI Adv. Mater.
PD OCT 12
PY 2016
VL 28
IS 38
BP 8405
EP 8412
DI 10.1002/adma.201601666
PG 8
WC Chemistry, Multidisciplinary; Chemistry, Physical; Nanoscience &
Nanotechnology; Materials Science, Multidisciplinary; Physics, Applied;
Physics, Condensed Matter
SC Chemistry; Science & Technology - Other Topics; Materials Science;
Physics
GA DZ8EM
UT WOS:000386103700008
PM 27454809
ER
PT J
AU Wu, WZ
Wang, L
Yu, RM
Liu, YY
Wei, SH
Hone, J
Wang, ZL
AF Wu, Wenzhuo
Wang, Lei
Yu, Ruomeng
Liu, Yuanyue
Wei, Su-Huai
Hone, James
Wang, Zhong Lin
TI Piezophototronic Effect in Single-Atomic-Layer MoS2 for Strain-Gated
Flexible Optoelectronics
SO ADVANCED MATERIALS
LA English
DT Article
DE adaptive optoelectronics; monolayer MoS2; piezophototronic effect
ID MONOLAYER MOS2; 2-DIMENSIONAL MATERIALS; PIEZO-PHOTOTRONICS;
ENERGY-CONVERSION; PIEZOTRONICS; LIGHT; DEVICES; PIEZOELECTRICITY;
ELECTRONICS; NANOSCALE
AB Strain-gated flexible optoelectronics are reported based on monolayer MoS2. Utilizing the piezoelectric polarization created at the metal-MoS2 interface to modulate the separation/transport of photo generated carriers, the piezophototronic effect is applied to implement atomic-layer-thick phototransistor. Coupling between piezoelectricity and photogenerated carriers may enable the development of novel optoelectronics.
C1 [Wu, Wenzhuo; Yu, Ruomeng; Wang, Zhong Lin] Georgia Inst Technol, Sch Mat Sci & Engn, Atlanta, GA 30332 USA.
[Wang, Lei] Columbia Univ, Dept Elect Engn, New York, NY 10027 USA.
[Liu, Yuanyue; Wei, Su-Huai] Natl Renewable Energy Lab, Golden, CO 80401 USA.
[Hone, James] Columbia Univ, Dept Mech Engn, New York, NY 10027 USA.
[Wang, Zhong Lin] Chinese Acad Sci, Beijing Inst Nanoenergy & Nanosyst, Beijing, Peoples R China.
RP Wang, ZL (reprint author), Georgia Inst Technol, Sch Mat Sci & Engn, Atlanta, GA 30332 USA.; Wang, ZL (reprint author), Chinese Acad Sci, Beijing Inst Nanoenergy & Nanosyst, Beijing, Peoples R China.
EM zhong.wang@mse.gatech.edu
RI Wang, Zhong Lin/E-2176-2011; Wu, Wenzhuo/G-1334-2010;
OI Wang, Zhong Lin/0000-0002-5530-0380; Wu, Wenzhuo/0000-0003-0362-6650;
Liu, Yuanyue/0000-0002-5880-8649
FU U.S. Department of Energy, Office of Basic Energy Sciences
[DE-FG02-07ER46394]; National Science Foundation [DMR-1505319,
DMR-1122594]; U.S. Department of Energy [DE-AC36-08GO28308]; Office of
Science of the U.S. Department of Energy [DE-AC02-05CH11231]; National
Natural Science Foundation of China [51432005]
FX W.Z.W., L.W., and R.M.Y. contributed equally to this work. This research
was supported by U.S. Department of Energy, Office of Basic Energy
Sciences (Award DE-FG02-07ER46394), the National Science Foundation
(DMR-1505319 and DMR-1122594). This work at NREL was supported by the
U.S. Department of Energy under Contract No. DE-AC36-08GO28308. This
work used the NREL Peregrine Supercomputer, and the National Energy
Research Scientific Computing Center (NERSC), which is supported by the
Office of Science of the U.S. Department of Energy under Contract No.
DE-AC02-05CH11231. Z.L.W. acknowledges the "Thousands Talents" program
for pioneer researcher and his innovation team, China and National
Natural Science Foundation of China (Grant No. 51432005). W.Z.W. and
Z.L.W. conceived the idea. W.Z.W., L.W., and Z.L.W. designed the
experiments. L.W. and J.H. prepared the materials. L.W. and W.Z.W.
fabricated the devices. W.Z.W., R.M.Y. and L.W. conducted the
experiments. Y.Y.L. and S.H.W. performed the first-principle
calculation. W.Z.W. and Z.L.W. analyzed the data and wrote the paper.
All authors discussed the results and commented on the paper.
NR 53
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U1 58
U2 58
PU WILEY-V C H VERLAG GMBH
PI WEINHEIM
PA POSTFACH 101161, 69451 WEINHEIM, GERMANY
SN 0935-9648
EI 1521-4095
J9 ADV MATER
JI Adv. Mater.
PD OCT 12
PY 2016
VL 28
IS 38
BP 8463
EP 8468
DI 10.1002/adma.201602854
PG 6
WC Chemistry, Multidisciplinary; Chemistry, Physical; Nanoscience &
Nanotechnology; Materials Science, Multidisciplinary; Physics, Applied;
Physics, Condensed Matter
SC Chemistry; Science & Technology - Other Topics; Materials Science;
Physics
GA DZ8EM
UT WOS:000386103700016
PM 27486923
ER
PT J
AU Yu, Y
Ludwig, KF
Woicik, JC
Gopalan, S
Pal, UB
Kaspar, TC
Basu, SN
AF Yu, Yang
Ludwig, Karl F.
Woicik, Joseph C.
Gopalan, Srikanth
Pal, Uday B.
Kaspar, Tiffany C.
Basu, Soumendra N.
TI Effect of Sr Content and Strain on Sr Surface Segregation of
La1-xSrxCo0.2Fe0.8O3-delta as Cathode Material for Solid Oxide Fuel
Cells
SO ACS APPLIED MATERIALS & INTERFACES
LA English
DT Article
DE solid oxide fuel cell; strontium-doped lanthanum cobalt ferrite; Sr
surface segregation; thin film; total-reflection X-ray fluorescence;
hard X-ray photoelectron spectroscopy; high-resolution X-ray diffraction
ID INTERMEDIATE TEMPERATURE SOFC; PEROVSKITE-TYPE OXIDES; COMPOSITE
CATHODES; ELECTRICAL-PROPERTIES; PERFORMANCE;
LA0.6SR0.4CO0.2FE0.8O3-DELTA; TRANSPORT; SYSTEM; FILMS;
LA0.6SR0.4COO3-DELTA
AB Strontium-doped lanthanum cobalt ferrite (LSCF) is a widely used cathode material due to its high electronic and ionic conductivity, and reasonable oxygen surface exchange coefficient. However, LSCF can have long-term stability issues such as surface segregation of Sr during solid oxide fuel cell (SOFC) operation, which can adversely affect the electrochemical performance. Thus, understanding the nature Of the Sr surface segregation phenomenon and how it is affected by the composition of LSCF and strain are critical. In this research, heteroepitaxial thin films of La1-xSrxCo0.2Fe0.8O3-delta with varying Sr content (x = 0.4, 0.3, 0.2) were deposited by pulsed laser deposition (PLD) on single-crystal NdGaO3, SrTiO3, and GdScO3 substrates, leading to different levels of strain in the films. The extent of Sr segregation at the film surface was quantified using synchrotron-based total-reflection X-ray fluorescence (TXRF) and atomic force microscopy (AFM). The electronic structure of the Sr-rich phases formed on the surface was investigated by hard X-ray photoelectron spectroscopy (HAXPES). The extent of Sr segregation was found to be a function of the Sr content in bulk. Lowering the Sr content from 40% to 30% reduced the surface segregation, but further lowering the Sr content to 20% increased the segregation. The strain of LSCF thin films on various" substrates was measured using high-resolution X-ray diffraction (HRXRD), and the Sr surface segregation was found to be reduced with compressive strain and enhanced with tensile strain present within the thin films. A model was developed correlating the Sr surface segregation with Sr content and strain effects to explain the experimental results.
C1 [Yu, Yang; Ludwig, Karl F.; Gopalan, Srikanth; Pal, Uday B.; Basu, Soumendra N.] Boston Univ, Div Mat Sci & Engn, Brookline, MA 02446 USA.
[Ludwig, Karl F.] Boston Univ, Dept Phys, 590 Commonwealth Ave, Boston, MA 02215 USA.
[Woicik, Joseph C.] NIST, Mat Measurement Lab, Gaithersburg, MD 20899 USA.
[Gopalan, Srikanth; Pal, Uday B.; Basu, Soumendra N.] Boston Univ, Dept Mech Engn, Boston, MA 02215 USA.
[Kaspar, Tiffany C.] Pacific Northwest Natl Lab, Div Phys Sci, Richland, WA 99354 USA.
RP Yu, Y; Basu, SN (reprint author), Boston Univ, Div Mat Sci & Engn, Brookline, MA 02446 USA.; Basu, SN (reprint author), Boston Univ, Dept Mech Engn, Boston, MA 02215 USA.
EM yuyang20@bu.edu; basu@bu.edu
FU DOE SECA program [DEFC2612FE0009656]; Office of Biological and
Environmental Research; U.S. Department of Energy, Office of Science,
Office of Basic Energy Sciences [DE-AC02-98CH10886]; National Institute
of Standards and Technology; NSF-MRI [1337471]
FX This work is supported through the DOE SECA program under Grant
DEFC2612FE0009656. Synthesis of materials was performed using EMSL, a
DOE Office of Science User Facility sponsored by the Office of
Biological and Environmental Research and located at Pacific Northwest
National Laboratory. Use of the National Synchrotron Light Source,
Brookhaven National Laboratory, was supported by the U.S. Department of
Energy, Office of Science, Office of Basic Energy Sciences, under
Contract No. DE-AC02-98CH10886. Additional support was provided by the
National Institute of Standards and Technology. The Bruker D8 Discover
diffractometer used for HRXRD studies was purchased through NSF-MRI
Award No. 1337471. The authors would like to acknowledge the
contributions of Mr. Barry Karlin at NIST, Dr. Jeff Bacon, Mr. Jeff
Woodward, and Dr. Alexey Y. Nikiforov at Boston University.
NR 49
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U1 25
U2 25
PU AMER CHEMICAL SOC
PI WASHINGTON
PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA
SN 1944-8244
J9 ACS APPL MATER INTER
JI ACS Appl. Mater. Interfaces
PD OCT 12
PY 2016
VL 8
IS 40
BP 26704
EP 26711
DI 10.1021/acsami.6b07118
PG 8
WC Nanoscience & Nanotechnology; Materials Science, Multidisciplinary
SC Science & Technology - Other Topics; Materials Science
GA DY9QD
UT WOS:000385469000031
PM 27649281
ER
PT J
AU Tian, LL
Li, SB
Zhang, MJ
Li, SK
Lin, LP
Zheng, JX
Zhuang, QC
Amine, K
Pan, F
AF Tian, Lei-Lei
Li, Si-Bai
Zhang, Ming-Jian
Li, Shuan-Kui
Lin, Ling-Piao
Zheng, Jia-Xin
Zhuang, Quan-Chao
Amine, Khalil
Pan, Feng
TI Cascading Boost Effect on the Capacity of Nitrogen-Doped Graphene Sheets
for Li- and Na-Ion Batteries
SO ACS APPLIED MATERIALS & INTERFACES
LA English
DT Article
DE nitrogen-doped graphene; cyclic performance; lithium ion battery; sodium
ion battery; first-principles calculation; capacity boost
ID OXYGEN REDUCTION REACTION; LITHIUM STORAGE; ANODE MATERIALS;
ENERGY-STORAGE; SINGLE-LAYER; RECHARGEABLE BATTERIES; ELECTRODE
MATERIALS; DEFECTIVE GRAPHENE; CARBON NANOTUBES; RATE CAPABILITY
AB Specific capacity and cyclic performance are critically important for the electrode materials of rechargeable batteries. Herein, a capacity boost effect of Li- and Na-ion batteries was presented and clarified by nitrogen-doped graphene sheets. The reversible capacities progressively increased from 637.4 to 1050.4 mAh g(-1) (164.8% increase) in Li-ion cell tests from 20 to 185 cycles, and from 187.3 to 247.5 mAh g(-1) (132.1% increase) in Na-ion cell tests from 50 to 500 cycles. The mechanism of the capacity boost is proposed as an electrochemical induced cascading evolution of graphitic N to pyridinic and/or pyrrolic N, during which only these graphitic N adjacent pyridinic or pyrrolic structures can be taken precedence. The original and new generated pyridinic and pyrrolic N have strengthened binding energies to Li/Na atoms, thus increased the Li/Na coverage and delivered a progressive capacity boost with cycles until the entire favorable graphitic N transform into pyridinic and pyrrolic N.
C1 [Tian, Lei-Lei; Li, Si-Bai; Zhang, Ming-Jian; Li, Shuan-Kui; Lin, Ling-Piao; Zheng, Jia-Xin; Amine, Khalil; Pan, Feng] Peking Univ, Shenzhen Grad Sch, Sch Adv Mat, Shenzhen 518055, Peoples R China.
[Zhuang, Quan-Chao] China Univ Min & Technol, Sch Mat Sci & Engn, Xuzhou 221116, Peoples R China.
[Amine, Khalil] Argonne Natl Lab, Chem Sci & Engn Div, Electrochem Technol Program, 9700 S Cass Ave, Argonne, IL 60439 USA.
RP Zheng, JX; Pan, F (reprint author), Peking Univ, Shenzhen Grad Sch, Sch Adv Mat, Shenzhen 518055, Peoples R China.; Zhuang, QC (reprint author), China Univ Min & Technol, Sch Mat Sci & Engn, Xuzhou 221116, Peoples R China.
EM zhengjx@pkusz.edu.cn; zhuangquanchao@126.com; panfeng@pkusz.edu.cn
RI Tian, Lei-Lei/H-9590-2012
OI Tian, Lei-Lei/0000-0001-5987-2944
FU Fund from the National Project for EV Batteries [20121110]; Guangdong
Innovation Team Project [2013N080]; Shenzhen Science and Technology
Research Grant [ZDSY20130331145131323, CXZZ20120829172325895,
JCYJ20150629144526408]; U.S. Department of Energy Office of Science
laboratory [DE-AC02-06CH11357]
FX The authors acknowledge financial support from the Fund from the
National Project for EV Batteries (20121110, Optimum Nano, Shenzhen),
the Guangdong Innovation Team Project (2013N080), and the Shenzhen
Science and Technology Research Grant (ZDSY20130331145131323,
CXZZ20120829172325895, and JCYJ20150629144526408). Argonne National
Laboratory, a U.S. Department of Energy Office of Science laboratory, is
operated under Contract DE-AC02-06CH11357. The authors are also grateful
to Dr. Hai-Biao Chen and Dr. Yi-Dong Liu for helpful discussions about
BET and XPS results.
NR 56
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U1 75
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PU AMER CHEMICAL SOC
PI WASHINGTON
PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA
SN 1944-8244
J9 ACS APPL MATER INTER
JI ACS Appl. Mater. Interfaces
PD OCT 12
PY 2016
VL 8
IS 40
BP 26722
EP 26729
DI 10.1021/acsami.6b07390
PG 8
WC Nanoscience & Nanotechnology; Materials Science, Multidisciplinary
SC Science & Technology - Other Topics; Materials Science
GA DY9QD
UT WOS:000385469000033
PM 27632809
ER
PT J
AU Schoedel, A
Li, M
Li, D
O'Keeffe, M
Yaghi, OM
AF Schoedel, Alexander
Li, Mian
Li, Dan
O'Keeffe, Michael
Yaghi, Omar M.
TI Structures of Metal-Organic Frameworks with Rod Secondary Building Units
SO CHEMICAL REVIEWS
LA English
DT Review
ID EARTH COORDINATION POLYMERS; SELECTIVE GAS-ADSORPTION; RAY-POWDER
DIFFRACTION; NANOSIZED TRIS((4-CARBOXYL)PHENYLDURYL)AMINE LIGAND;
CARBON-DIOXIDE ADSORPTION; SLOW MAGNETIC-RELAXATION; CUBIC CYLINDER
PACKINGS; BOERDIJK-COXETER HELIX; HIGH-SURFACE-AREA; IN-SILICO DESIGN
AB Rod MOFs are metal organic frameworks in which the metal-containing secondary building units consist of infinite rods of linked metal-centered polyhedra. For such materials, we identify the points of extension, often atoms, which define the interface between the organic and inorganic components of the structure. The pattern of points of extension defines a shape such as a helix, ladder, helical ribbon, or cylinder tiling. The linkage of these shapes into a three-dimensional framework in turn defines a net characteristic of the original structure. Some scores of rod MOF structures are illustrated and deconstructed into their underlying nets in this way. Crystallographic data for all nets in their maximum symmetry embeddings are provided.
C1 [Schoedel, Alexander; Yaghi, Omar M.] Univ Calif Berkeley, Dept Chem, Berkeley, CA 94720 USA.
[Schoedel, Alexander; Yaghi, Omar M.] Lawrence Berkeley Natl Lab, Kavli Energy Nanosci Inst, Div Mat Sci, Berkeley, CA 94720 USA.
[Schoedel, Alexander] Florida Inst Technol, Dept Chem, 150 West Univ Blvd, Melbourne, FL 32901 USA.
[Li, Mian; Li, Dan] Shantou Univ, Dept Chem, Shantou 515063, Guangdong, Peoples R China.
[Li, Dan] Jinan Univ, Coll Chem & Mat Sci, Guangzhou 510632, Guangdong, Peoples R China.
[O'Keeffe, Michael] Arizona State Univ, Sch Mol Sci, Tempe, AZ 85287 USA.
[Yaghi, Omar M.] King Abdulaziz City Sci & Technol, POB 6086, Riyadh 11442, Saudi Arabia.
RP O'Keeffe, M (reprint author), Arizona State Univ, Sch Mol Sci, Tempe, AZ 85287 USA.
EM mokeeffe@asu.edu
RI Li, Dan/F-2708-2014; Schoedel, Alexander/B-3971-2013;
OI Schoedel, Alexander/0000-0001-6548-9300; Yaghi,
Omar/0000-0002-5611-3325; Li, Mian/0000-0003-1293-3636
FU BASF SE (Ludwigshafen, Germany); U.S. Department of Defense; Defense
Threat Reduction Agency [HDTRA 1-12-10053]; U.S. Department of Energy,
Office of Science, Office of Basic Energy Sciences, Energy Frontier
Research Center [DE-SC0001015]; US National Science Foundation [DMR
1104798]; National Basic Research Program of China (973 Program)
[2012CB821706, 2013CB834803]; National Natural Science Foundation of
China [91222202, 21171114]; German Research Foundation (DFG) [SCHO
1639/1-1]
FX Funding of MOF research in the Omar Yaghi group is supported by BASF SE
(Ludwigshafen, Germany), U.S. Department of Defense, Defense Threat
Reduction Agency (HDTRA 1-12-10053), U.S. Department of Energy, Office
of Science, Office of Basic Energy Sciences, Energy Frontier Research
Center grant (DE-SC0001015). Michael O'Keeffe's research is supported by
the US National Science Foundation, grant DMR 1104798. Funding of MOF
research in the Dan Li group is supported by the National Basic Research
Program of China (973 Program, 2012CB821706 and 2013CB834803) and the
National Natural Science Foundation of China (91222202 and 21171114).
A.S. gratefully acknowledges the German Research Foundation (DFG, SCHO
1639/1-1) for financial support. We thank Ms. Noelle Catarineu for
fruitful discussions on MOF-910.
NR 274
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U1 179
U2 179
PU AMER CHEMICAL SOC
PI WASHINGTON
PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA
SN 0009-2665
EI 1520-6890
J9 CHEM REV
JI Chem. Rev.
PD OCT 12
PY 2016
VL 116
IS 19
BP 12466
EP 12535
DI 10.1021/acs.chemrev.6b00346
PG 70
WC Chemistry, Multidisciplinary
SC Chemistry
GA DY9QF
UT WOS:000385469400018
PM 27627623
ER
PT J
AU Zhang, DD
Yu, Y
Bekenstein, Y
Wong, AB
Alivisatos, AP
Yang, PD
AF Zhang, Dandan
Yu, Yi
Bekenstein, Yehonadav
Wong, Andrew B.
Alivisatos, A. Paul
Yang, Peidong
TI Ultrathin Colloidal Cesium Lead Halide Perovskite Nanowires
SO JOURNAL OF THE AMERICAN CHEMICAL SOCIETY
LA English
DT Article
ID SOLUTION-PHASE; NANOCRYSTALS; EXCHANGE; BINDING
AB Highly uniform single crystal ultrathin CsPbBr3 nanowires (NWs) with diameter of 2.2 +/- 0.2 nm and length up to several microns were successfully synthesized and purified using a catalyst-free colloidal synthesis method followed by a stepwise purification strategy. The NWs have bright photoluminescence (PL) with a photoluminescence quantum yield (PLQY) of about 30% after surface treatment. Large blue-shifted UV-vis absorption and PL spectra have been observed due to strong two-dimensional quantum confinement effects. A small angle X-ray scattering (SAXS) pattern shows the periodic packing of the ultrathin NWs along the radial direction, demonstrates the narrow radial distribution of the wires, and emphasizes the deep intercalation of the surfactants. Despite the extreme aspect ratios of the ultrathin NWs, their composition and the resulting optical properties can be readily tuned by an anion-exchange reaction with good morphology preservation. These bright ultrathin NWs may be used as a model system to study strong quantum confinement effects in a one-dimensional halide perovskite system.
C1 [Zhang, Dandan; Yu, Yi; Bekenstein, Yehonadav; Wong, Andrew B.; Alivisatos, A. Paul; Yang, Peidong] Univ Calif Berkeley, Dept Chem, Berkeley, CA 94720 USA.
[Alivisatos, A. Paul; Yang, Peidong] Univ Calif Berkeley, Dept Mat Sci & Engn, Berkeley, CA 94720 USA.
[Zhang, Dandan; Yu, Yi; Bekenstein, Yehonadav; Wong, Andrew B.; Alivisatos, A. Paul; Yang, Peidong] Lawrence Berkeley Natl Lab, Div Mat Sci, Berkeley, CA 94720 USA.
[Bekenstein, Yehonadav; Alivisatos, A. Paul; Yang, Peidong] Kavli Energy NanoSci Inst, Berkeley, CA 94720 USA.
RP Yang, PD (reprint author), Univ Calif Berkeley, Dept Chem, Berkeley, CA 94720 USA.; Yang, PD (reprint author), Univ Calif Berkeley, Dept Mat Sci & Engn, Berkeley, CA 94720 USA.; Yang, PD (reprint author), Lawrence Berkeley Natl Lab, Div Mat Sci, Berkeley, CA 94720 USA.; Yang, PD (reprint author), Kavli Energy NanoSci Inst, Berkeley, CA 94720 USA.
EM p_yang@berkeley.edu
RI Alivisatos , Paul /N-8863-2015
OI Alivisatos , Paul /0000-0001-6895-9048
FU Physical Chemistry of Inorganic Nanostructures Program [KC3103]; Office
of Basic Energy Sciences of the United States Department of Energy
[DE-AC02-05CH11231]; Office of Science, Office of Basic Energy Sciences
of the U.S. Department of Energy [DE-AC02-05CH11231]; Suzhou Industrial
Park; LAM Research Fellowship
FX This work was supported by the Physical Chemistry of Inorganic
Nanostructures Program, KC3103, Office of Basic Energy Sciences of the
United States Department of Energy under Contract No. DE-AC02-05CH11231.
Work at the NCEM, Molecular Foundry was supported by the Office of
Science, Office of Basic Energy Sciences of the U.S. Department of
Energy under Contract No. DE-AC02-05CH11231. D.Z. would like to
acknowledge the fellowship support from Suzhou Industrial Park. A.B.W.
would like to acknowledge the support of the LAM Research Fellowship.
NR 24
TC 8
Z9 8
U1 71
U2 71
PU AMER CHEMICAL SOC
PI WASHINGTON
PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA
SN 0002-7863
J9 J AM CHEM SOC
JI J. Am. Chem. Soc.
PD OCT 12
PY 2016
VL 138
IS 40
BP 13155
EP 13158
DI 10.1021/jacs.6b08373
PG 4
WC Chemistry, Multidisciplinary
SC Chemistry
GA DY9QG
UT WOS:000385469600015
PM 27673493
ER
PT J
AU Heine, C
Lechner, BAJ
Bluhm, H
Salmeron, M
AF Heine, Christian
Lechner, Barbara A. J.
Bluhm, Hendrik
Salmeron, Miquel
TI Recycling of CO2: Probing the Chemical State of the Ni(111) Surface
during the Methanation Reaction with Ambient-Pressure X-Ray
Photoelectron Spectroscopy
SO JOURNAL OF THE AMERICAN CHEMICAL SOCIETY
LA English
DT Article
ID CARBON-DIOXIDE HYDROGENATION; NICKEL METAL; OXYGEN; CATALYSTS; NI(100);
OXIDE; GAS; XPS; CHEMISORPTION; MECHANISMS
AB Using ambient-pressure X-ray photoelectron spectroscopy (AP-XPS), we studied the adsorption and reactions of CO2 and CO2 + H-2 on the Ni(111) surface to identify the surface chemical state and the nature of the adsorbed species during the methanation reaction. In 200 mTorr CO2, we found that NiO is formed from CO2 dissociation into CO and atomic oxygen. Additionally, carbonate (CO32-) is present on the surface from further reaction of CO2 with NiO. The addition of H-2 into the reaction environment leads to reduction of NiO and the disappearance of CO32-. At temperatures >160 degrees C, CO adsorbed on hollow sites, and atomic carbon and OH species are present on the surface. We conclude that the methanation reaction proceeds via dissociation of CO2, followed by reduction of CO to atomic carbon and its hydrogenation to methane.
C1 [Heine, Christian; Lechner, Barbara A. J.; Salmeron, Miquel] Lawrence Berkeley Natl Lab, Mat Sci, 1 Cyclotron Rd, Berkeley, CA 94720 USA.
[Bluhm, Hendrik] Lawrence Berkeley Natl Lab, Div Chem Sci, 1 Cyclotron Rd, Berkeley, CA 94720 USA.
[Salmeron, Miquel] Univ Calif Berkeley, Dept Mat Sci & Engn, Berkeley, CA 94720 USA.
[Lechner, Barbara A. J.] Tech Univ Munich, Dept Chem, Lichtenbergstr 4, D-85748 Garching, Germany.
RP Salmeron, M (reprint author), Lawrence Berkeley Natl Lab, Mat Sci, 1 Cyclotron Rd, Berkeley, CA 94720 USA.; Salmeron, M (reprint author), Univ Calif Berkeley, Dept Mat Sci & Engn, Berkeley, CA 94720 USA.
EM mbsalmeron@lbl.gov
FU Integrated Mesoscale Architectures for Sustainable Catalysis (IMASC), an
Energy Frontier Research Center - U.S. Department of Energy (DOE),
Office of Science, Basic Energy Sciences [DE-SC0012573]; Office of
Science of the U.S. DOE [DE-AC02-05CH11231]
FX This work was supported by the Integrated Mesoscale Architectures for
Sustainable Catalysis (IMASC), an Energy Frontier Research Center funded
by the U.S. Department of Energy (DOE), Office of Science, Basic Energy
Sciences, under Award No. DE-SC0012573. It used resources of the Advance
Light Source, a user Facility supported by the Office of Science of the
U.S. DOE under Contract DE-AC02-05CH11231.
NR 53
TC 1
Z9 1
U1 31
U2 31
PU AMER CHEMICAL SOC
PI WASHINGTON
PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA
SN 0002-7863
J9 J AM CHEM SOC
JI J. Am. Chem. Soc.
PD OCT 12
PY 2016
VL 138
IS 40
BP 13246
EP 13252
DI 10.1021/jacs.6b06939
PG 7
WC Chemistry, Multidisciplinary
SC Chemistry
GA DY9QG
UT WOS:000385469600029
PM 27599672
ER
PT J
AU Zheng, JX
Liu, TC
Hu, ZX
Wei, Y
Song, XH
Ren, Y
Wang, WD
Rao, MM
Lin, Y
Chen, ZH
Lu, J
Wang, CM
Amine, K
Pan, F
AF Zheng, Jiaxin
Liu, Tongchao
Hu, Zongxiang
Wei, Yi
Song, Xiaohe
Ren, Yang
Wang, Weidong
Rao, Mumin
Lin, Yuan
Chen, Zonghai
Lu, Jun
Wang, Chongmin
Amine, Khalil
Pan, Feng
TI Tuning of Thermal Stability in Layered Li(NixMnyCoz)O-2
SO JOURNAL OF THE AMERICAN CHEMICAL SOCIETY
LA English
DT Article
ID LITHIUM-ION BATTERIES; TIME-RESOLVED XRD; TOTAL-ENERGY CALCULATIONS;
AUGMENTED-WAVE METHOD; CATHODE MATERIALS; ELECTROCHEMICAL PROPERTIES;
STRUCTURAL-CHANGES; NONAQUEOUS ELECTROLYTE; HIGH-CAPACITY; BASIS-SET
AB Understanding and further designing new layered Li(NixMnyCoz)O-2 (NMC) (x + y + z = 1) materials with optimized thermal stability is important to rechargeable Li batteries (LIBs) for electrical vehicles (EV). Using ab initio calculations combined with experiments, we clarified how the thermal stability of NMC materials can be tuned by the most unstable oxygen, which is determined by the local coordination structure unit (LCSU) of oxygen (TM(Ni, Mn, Co)(3)-O-Li3-x'): each O atom bonds with three transition metals (TM) from the TM-layer and three to zero Li from fully discharged to charged states from the Li-layer. Under this model, how the lithium content, valence states of Ni, contents of Ni, Mn, and Co, and Ni/Li disorder to tune the thermal stability of NMC materials by affecting the sites, content, and the release temperature of the most unstable oxygen is proposed. The synergistic effect between Li vacancies and raised valence state of Ni during delithiation process can aggravate instability of oxygen, and oxygen coordinated with more nickel (especially with high valence state) in LSCU becomes more unstable at a fixed delithiation state. The Ni/Li mixing would decrease the thermal stability of the "Ni=Mn" group NMC materials but benefit the thermal stability of "Ni-rich" group, because the Ni in the Li layer would form 180 degrees Ni-O-Ni super exchange chains in "Ni-rich" NMC materials. Mn and Co doping can tune the initial valence state of Ni, local coordination environment of oxygen, and the Ni/Li disorder, thus to tune the thermal stability directly.
C1 [Zheng, Jiaxin; Liu, Tongchao; Hu, Zongxiang; Wei, Yi; Song, Xiaohe; Lin, Yuan; Pan, Feng] Peking Univ, Shenzhen Grad Sch, Sch Adv Mat, Shenzhen 518055, Peoples R China.
[Ren, Yang; Chen, Zonghai; Lu, Jun; Amine, Khalil] Argonne Natl Lab, Chem Sci & Engn Div, Electrochem Technol Program, Argonne, IL 60439 USA.
[Wang, Weidong] Shenzhen Tianjiao Technol Dev Co Ltd, Shenzhen 518119, Peoples R China.
[Rao, Mumin] Shenzhen OptimumNano Energy Co Ltd, Shenzhen 518118, Peoples R China.
[Wang, Chongmin] Pacific Northwest Natl Lab, Environm Mol Sci Lab, 902 Battelle Blvd, Richland, WA 99352 USA.
RP Pan, F (reprint author), Peking Univ, Shenzhen Grad Sch, Sch Adv Mat, Shenzhen 518055, Peoples R China.
EM panfeng@pkusz.edu.cn
RI lin, yuan/G-9390-2013
OI lin, yuan/0000-0003-3410-3588
FU National Materials Genome Project [2016YFB0700600]; National Project for
EV Batteries [20121110]; Guangdong Innovation Team Project [2013N080];
Shenzhen Science and Technology Research Grant [ZDSY20130331145131323,
JCYJ20140903101633318, JCYJ2014090-3101617271]; U.S. Department of
Energy, Office of Science, Office of Basic Energy Science
FX The work was financially supported by National Materials Genome Project
(2016YFB0700600), National Project for EV Batteries (20121110,
OptimumNano, Shenzhen), Guangdong Innovation Team Project (no.
2013N080), Shenzhen Science and Technology Research Grant (nos.
ZDSY20130331145131323, JCYJ20140903101633318, JCYJ2014090-3101617271).
The authors also acknowledge the use of the Advanced Photon Source
(APS), which is supported by the U.S. Department of Energy, Office of
Science, Office of Basic Energy Science.
NR 55
TC 2
Z9 2
U1 73
U2 73
PU AMER CHEMICAL SOC
PI WASHINGTON
PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA
SN 0002-7863
J9 J AM CHEM SOC
JI J. Am. Chem. Soc.
PD OCT 12
PY 2016
VL 138
IS 40
BP 13326
EP 13334
DI 10.1021/jacs.6b07771
PG 9
WC Chemistry, Multidisciplinary
SC Chemistry
GA DY9QG
UT WOS:000385469600038
PM 27642806
ER
PT J
AU Mackrory, JB
Bhattacharya, T
Steck, DA
AF Mackrory, Jonathan B.
Bhattacharya, Tanmoy
Steck, Daniel A.
TI Worldline approach for numerical computation of electromagnetic Casimir
energies: Scalar field coupled to magnetodielectric media
SO PHYSICAL REVIEW A
LA English
DT Article
ID DIELECTRICS; QUANTIZATION; ELECTRODYNAMICS
AB We present a worldline method for the calculation of Casimir energies for scalar fields coupled to magnetodielectricmedia. The scalar model we consider may be applied in arbitrary geometries, and it corresponds exactly to one polarization of the electromagnetic field in planar layered media. Starting from the field theory for electromagnetism, we work with the two decoupled polarizations in planar media and develop worldline path integrals, which represent the two polarizations separately, for computing both Casimir and Casimir-Polder potentials. We then show analytically that the path integrals for the transverse-electric polarization coupled to a dielectricmedium converge to the proper solutions in certain special cases, including the Casimir-Polder potential of an atom near a planar interface, and the Casimir energy due to two planar interfaces. We also evaluate the path integrals numerically viaMonte Carlo path-averaging for these cases, studying the convergence and performance of the resulting computational techniques. While these scalar methods are only exact in particular geometries, they may serve as an approximation for Casimir energies for the vector electromagnetic field in other geometries.
C1 [Mackrory, Jonathan B.; Steck, Daniel A.] Dept Phys, 1274 Univ Oregon, Eugene, OR 97403 USA.
[Mackrory, Jonathan B.; Steck, Daniel A.] Oregon Ctr Opt Mol & Quantum Sci, 1274 Univ Oregon, Eugene, OR 97403 USA.
[Bhattacharya, Tanmoy] Santa Fe Inst, Santa Fe, NM 87501 USA.
[Bhattacharya, Tanmoy] Los Alamos Natl Lab, Theoret Div T2, Los Alamos, NM 87545 USA.
RP Mackrory, JB (reprint author), Dept Phys, 1274 Univ Oregon, Eugene, OR 97403 USA.; Mackrory, JB (reprint author), Oregon Ctr Opt Mol & Quantum Sci, 1274 Univ Oregon, Eugene, OR 97403 USA.
FU NSF [PHY-1068583, PHY-1505118]
FX The authors thank Richard Wagner and Wes Erickson for comments on the
manuscript. This research was supported by NSF Grants No. PHY-1068583
and No. PHY-1505118.
NR 61
TC 0
Z9 0
U1 2
U2 2
PU AMER PHYSICAL SOC
PI COLLEGE PK
PA ONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA
SN 2469-9926
EI 2469-9934
J9 PHYS REV A
JI Phys. Rev. A
PD OCT 12
PY 2016
VL 94
IS 4
AR 042508
DI 10.1103/PhysRevA.94.042508
PG 20
WC Optics; Physics, Atomic, Molecular & Chemical
SC Optics; Physics
GA DZ1RW
UT WOS:000385618000004
ER
PT J
AU Moussa, JE
AF Moussa, Jonathan E.
TI Transversal Clifford gates on folded surface codes
SO PHYSICAL REVIEW A
LA English
DT Article
ID TOLERANT QUANTUM COMPUTATION; SYSTEMS; ANYONS; MEMORY; MODEL
AB Surface and color codes are two forms of topological quantum error correction in two spatial dimensions with complementary properties. Surface codes have lower-depth error detection circuits and well-developed decoders to interpret and correct errors, while color codes have transversal Clifford gates and better code efficiency in the number of physical qubits needed to achieve a given code distance. A formal equivalence exists between color codes and folded surface codes, but it does not guarantee the transferability of any of these favorable properties. However, the equivalence does imply the existence of constant-depth circuit implementations of logical Clifford gates on folded surface codes. We achieve and improve this result by constructing two families of folded surface codes with transversal Clifford gates. This construction is presented generally for qudits of any dimension. The specific application of these codes to universal quantum computation based on qubit fusion is also discussed.
C1 [Moussa, Jonathan E.] Sandia Natl Labs, Ctr Res Comp, Albuquerque, NM 87185 USA.
RP Moussa, JE (reprint author), Sandia Natl Labs, Ctr Res Comp, Albuquerque, NM 87185 USA.
EM godotalgorithm@gmail.com
FU Laboratory Directed Research and Development program at Sandia National
Laboratories; U.S. Department of Energy's National Nuclear Security
Administration [DE-AC04-94AL85000]
FX I thank Ciaran Ryan-Anderson for useful discussions. This work was
supported by the Laboratory Directed Research and Development program at
Sandia National Laboratories. Sandia National Laboratories is a
multiprogram laboratory managed and operated by Sandia Corporation, a
wholly owned subsidiary of Lockheed Martin Corporation, for the U.S.
Department of Energy's National Nuclear Security Administration under
contract DE-AC04-94AL85000.
NR 45
TC 1
Z9 1
U1 4
U2 4
PU AMER PHYSICAL SOC
PI COLLEGE PK
PA ONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA
SN 2469-9926
EI 2469-9934
J9 PHYS REV A
JI Phys. Rev. A
PD OCT 12
PY 2016
VL 94
IS 4
AR 042316
DI 10.1103/PhysRevA.94.042316
PG 14
WC Optics; Physics, Atomic, Molecular & Chemical
SC Optics; Physics
GA DZ1RW
UT WOS:000385618000002
ER
PT J
AU Sarkisov, GS
Rosenthal, SE
Struve, KW
AF Sarkisov, G. S.
Rosenthal, S. E.
Struve, K. W.
TI Dynamic polarizability of tungsten atoms reconstructed from fast
electrical explosion of fine wires in vacuum
SO PHYSICAL REVIEW A
LA English
DT Article
AB Nanosecond electrical explosion of fine metal wires in vacuum generates calibrated, radially expanded gas cylinders of metal atoms surrounded by a low-density fast expanding plasma corona. An integrated-phase technique, based on laser interferometry, provides the dynamic dipole polarizability of metal atoms. These data were previously unavailable for tungsten atoms. An extremely high melting temperature and significant premelt electronic emission make these measurements particularly complicated for this refractory metal. Most attempts to vaporize tungsten wire by electrical current pulse result in the disintegration of the sample into macro- and microfragments. However, application of a very fast-rising current, similar to 1 kA/ns, can vaporize a thin 10-15 mu m-diameter tungsten wire and generate a calibrated gas-plasma cylinder. Adding a dielectric coating to the wire leads to increased energy deposition to the wire core and a reduction of the surrounding plasma corona. Employing the integrated-phase technique on a fast-exploding coated tungsten wire, we find that the dynamic dipole polarizability of tungsten atoms at a wavelength of 532 nm equals 15 +/- 1.3 angstrom(3).
C1 [Sarkisov, G. S.] Raytheon Ktech, 1300 Eubank Blvd, Albuquerque, NM 87123 USA.
[Rosenthal, S. E.; Struve, K. W.] Sandia Natl Labs, Albuquerque, NM 87110 USA.
RP Sarkisov, GS (reprint author), Raytheon Ktech, 1300 Eubank Blvd, Albuquerque, NM 87123 USA.
FU National Nuclear Security Administration [DE-AC04-94AL85000]
FX Sandia is a multiprogram laboratory operated by Sandia Corporation, a
Lockheed Martin Company, for the National Nuclear Security
Administration under Contract No. DE-AC04-94AL85000.
NR 12
TC 0
Z9 0
U1 7
U2 7
PU AMER PHYSICAL SOC
PI COLLEGE PK
PA ONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA
SN 2469-9926
EI 2469-9934
J9 PHYS REV A
JI Phys. Rev. A
PD OCT 12
PY 2016
VL 94
IS 4
AR 042509
DI 10.1103/PhysRevA.94.042509
PG 5
WC Optics; Physics, Atomic, Molecular & Chemical
SC Optics; Physics
GA DZ1RW
UT WOS:000385618000005
ER
PT J
AU Bekaert, J
Vercauteren, S
Aperis, A
Komendova, L
Prozorov, R
Partoens, B
Milosevic, MV
AF Bekaert, J.
Vercauteren, S.
Aperis, A.
Komendova, L.
Prozorov, R.
Partoens, B.
Milosevic, M. V.
TI Anisotropic type-I superconductivity and anomalous superfluid density in
OsB2
SO PHYSICAL REVIEW B
LA English
DT Article
ID TEMPERATURE; LATTICE; METALS; MGB2
AB We present a microscopic study of superconductivity in OsB2, and discuss the origin and characteristic length scales of the superconducting state. From first-principles we show that OsB2 is characterized by three different Fermi sheets, and we prove that this fermiology complies with recent quantum-oscillation experiments. Using the found microscopic properties, and experimental data from the literature, we employ Ginzburg-Landau relations to reveal that OsB2 is a distinctly type-I superconductor with a very low Ginzburg-Landau parameter kappa-a rare property among compound materials. We show that the found coherence length and penetration depth corroborate the measured thermodynamic critical field. Moreover, our calculation of the superconducting gap structure using anisotropic Eliashberg theory and ab initio calculated electron-phonon interaction as input reveals a single but anisotropic gap. The calculated gap spectrum is shown to give an excellent account for the unconventional behavior of the superfluid density of OsB2 measured in experiments as a function of temperature. This reveals that gap anisotropy can explain such behavior, observed in several compounds, which was previously attributed solely to a two-gap nature of superconductivity.
C1 [Bekaert, J.; Vercauteren, S.; Komendova, L.; Partoens, B.; Milosevic, M. V.] Univ Antwerp, Dept Phys, Condensed Matter Theory Grp, Groenenborgerlaan 171, B-2020 Antwerp, Belgium.
[Aperis, A.; Komendova, L.] Uppsala Univ, Dept Phys & Astron, POB 516, SE-75120 Uppsala, Sweden.
[Prozorov, R.] Iowa State Univ, Dept Phys & Astron, Ames, IA 50011 USA.
[Prozorov, R.] Iowa State Univ, Ames Lab, Ames, IA 50011 USA.
RP Bekaert, J (reprint author), Univ Antwerp, Dept Phys, Condensed Matter Theory Grp, Groenenborgerlaan 171, B-2020 Antwerp, Belgium.
EM jonas.bekaert@uantwerpen.be; milorad.milosevic@uantwerpen.be
RI Milosevic, Milorad/H-9393-2012
FU TOPBOF-UAntwerp; Research Foundation-Flanders (FWO); COST action
[MP1201]; Swedish Research Council (Vetenskapsradet); Hercules
foundation; Flemish Government (EWI Department)
FX This work was supported by TOPBOF-UAntwerp, Research Foundation-Flanders
(FWO) and COST action MP1201. A.A. and L.K. acknowledge funding from the
Swedish Research Council (Vetenskapsradet). L.K. also acknowledges the
Wenner-Gren Foundations. The first-principles calculations were carried
out on the HPC infrastructure of the University of Antwerp (CalcUA), a
division of the Flemish Supercomputer Centre (VSC), supported
financially by the Hercules foundation and the Flemish Government (EWI
Department). The anisotropic Eliashberg calculations were performed
using resources from the Swedish National Infrastructure for Computing
(SNIC).
NR 45
TC 1
Z9 1
U1 2
U2 2
PU AMER PHYSICAL SOC
PI COLLEGE PK
PA ONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA
SN 2469-9950
EI 2469-9969
J9 PHYS REV B
JI Phys. Rev. B
PD OCT 12
PY 2016
VL 94
IS 14
AR 144506
DI 10.1103/PhysRevB.94.144506
PG 9
WC Physics, Condensed Matter
SC Physics
GA DZ1TF
UT WOS:000385622500009
ER
PT J
AU Li, L
Cao, HB
Parker, DS
Kuhn, SJ
Sefat, AS
AF Li, Li
Cao, Huibo
Parker, David S.
Kuhn, Stephen J.
Sefat, Athena S.
TI Persistent magnetism in silver-doped BaFe2As2 crystals
SO PHYSICAL REVIEW B
LA English
DT Article
ID IRON-BASED SUPERCONDUCTORS; HIGH-TEMPERATURE SUPERCONDUCTIVITY;
ELECTRONIC-STRUCTURE; CHALCOGENIDES; NEUTRON; FE
AB We investigate the thermodynamic and transport properties of silver-substituted BaFe2As2 (122) crystals up to similar to 4.5%. Similar to other transition-metal substitutions in 122, Ag diminishes the antiferromagnetic (T-N) and structural (T-S) transition temperatures, but unlike other electron-doped 122s, T-N and T-S coincide without splitting. Although magnetism drops precipitously to T-N = 84K at doping x = 0.029, it only weakly changes above this x, settling at T-N = 80K at x = 0.045. Compared to this persistent magnetism in Ag-122, doping other group 11 elements of either Cu or Au in 122 diminished T-N and induced superconductivity near T-c = 2K at x = 0.044 or 0.031, respectively. Ag-122 crystals show reflective surfaces with surprising thicker cross sections for x >= 0.019, the appearance that is in contrast to the typical thin stacked layered feature seen in all other flux-grown x122 and lower Ag-122. This physical trait may be a manifest of intrinsic weak changes in c lattice and T-N. Our theoretical calculations suggest that Ag doping produces strong electronic scattering and yet a relatively small disruption of the magnetic state, both of which preclude superconductivity in this system.
C1 [Li, Li; Parker, David S.; Kuhn, Stephen J.; Sefat, Athena S.] Oak Ridge Natl Lab, Div Mat Sci & Technol, Oak Ridge, TN 37831 USA.
[Cao, Huibo] Oak Ridge Natl Lab, Quantum Condensed Matter Div, Oak Ridge, TN 37831 USA.
[Kuhn, Stephen J.] Univ Notre Dame, Dept Phys, Notre Dame, IN 46556 USA.
RP Li, L (reprint author), Oak Ridge Natl Lab, Div Mat Sci & Technol, Oak Ridge, TN 37831 USA.
RI Sefat, Athena/R-5457-2016
OI Sefat, Athena/0000-0002-5596-3504
FU U.S. Department of Energy (DOE), Office of Science, Basic Energy
Sciences, Materials Science and Engineering Division; Scientific User
Facilities Division, Office of Basic Energy Sciences, U.S. DOE; DOE
Office of Science Graduate Student Research Program [DE-AC05-06OR23100]
FX This paper was primarily supported by the U.S. Department of Energy
(DOE), Office of Science, Basic Energy Sciences, Materials Science and
Engineering Division (L.L., D.S.P., A.S.S.). The paper at ORNL's HFIR
(H.C.) was sponsored by the Scientific User Facilities Division, Office
of Basic Energy Sciences, U.S. DOE. S.K. would like to acknowledge DOE
Office of Science Graduate Student Research Program award for funding
under Contract No. DE-AC05-06OR23100.
NR 61
TC 0
Z9 0
U1 6
U2 6
PU AMER PHYSICAL SOC
PI COLLEGE PK
PA ONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA
SN 2469-9950
EI 2469-9969
J9 PHYS REV B
JI Phys. Rev. B
PD OCT 12
PY 2016
VL 94
IS 13
AR 134510
DI 10.1103/PhysRevB.94.134510
PG 8
WC Physics, Condensed Matter
SC Physics
GA DZ1SO
UT WOS:000385620300007
ER
PT J
AU Tsesmetzis, N
Yilmaz, P
Marks, PC
Kyrpides, NC
Head, IM
Lomans, BP
AF Tsesmetzis, Nicolas
Yilmaz, Pelin
Marks, Peter C.
Kyrpides, Nikos C.
Head, Ian M.
Lomans, Bart P.
TI MIxS-HCR: a MIxS extension defining a minimal information standard for
sequence data from environments pertaining to hydrocarbon resources
SO STANDARDS IN GENOMIC SCIENCES
LA English
DT Article
DE Hydrocarbon resources; Sequence data; MIxS standards; Environmental
package
ID TEMPERATURE PETROLEUM RESERVOIR; PHYLOGENETIC DIVERSITY; MICROBIAL
COMMUNITY; WATER; BACTERIA
AB Here we introduce a MIxS extension to facilitate the recording and cataloguing of metadata from samples related to hydrocarbon resources. The proposed MIxS-HCR package incorporates the core features of the MIxS standard for marker gene (MIMARKS) and metagenomic (MIMS) sequences along with a hydrocarbon resources customized environmental package. Adoption of the MIxS-HCR standard will enable the comparison and better contextualization of investigations related to hydrocarbon rich environments. The insights from such standardized way of reporting could be highly beneficial for the successful development and optimization of hydrocarbon recovery processes and management of microbiological issues in petroleum production systems.
C1 [Tsesmetzis, Nicolas; Marks, Peter C.] Shell Int Explorat & Prod Inc, 3333 HW6S, Houston, TX 77082 USA.
[Yilmaz, Pelin] Max Planck Inst Marine Microbiol, Microbial Genom & Bioinformat Res Grp, Bremen, Germany.
[Kyrpides, Nikos C.] DOE Joint Genome Inst, Walnut Creek, CA 94598 USA.
[Head, Ian M.] Newcastle Univ, Sch Civil Engn & Geosci, Newcastle Upon Tyne NE1 7RU, Tyne & Wear, England.
[Lomans, Bart P.] Shell Global Solut Int BV, Rijswijk, Netherlands.
RP Tsesmetzis, N (reprint author), Shell Int Explorat & Prod Inc, 3333 HW6S, Houston, TX 77082 USA.
EM nicolas.tsesmetzis@shell.com
RI Kyrpides, Nikos/A-6305-2014;
OI Kyrpides, Nikos/0000-0002-6131-0462; Head, Ian/0000-0002-5373-162X
FU Royal Dutch Shell
FX This work was partly funded by Royal Dutch Shell.
NR 16
TC 0
Z9 0
U1 2
U2 2
PU BIOMED CENTRAL LTD
PI LONDON
PA 236 GRAYS INN RD, FLOOR 6, LONDON WC1X 8HL, ENGLAND
SN 1944-3277
J9 STAND GENOMIC SCI
JI Stand. Genomic Sci.
PD OCT 12
PY 2016
VL 11
AR 78
DI 10.1186/s40793-016-0203-5
PG 6
WC Genetics & Heredity; Microbiology
SC Genetics & Heredity; Microbiology
GA DY7OD
UT WOS:000385317700001
PM 27777648
ER
PT J
AU Fang, L
Im, J
DeGottardi, W
Jia, Y
Glatz, A
Matveev, KA
Kwok, WK
Crabtree, GW
Kanatzidis, MG
AF Fang, L.
Im, J.
DeGottardi, W.
Jia, Y.
Glatz, A.
Matveev, K. A.
Kwok, W. -K.
Crabtree, G. W.
Kanatzidis, M. G.
TI Large spin-orbit coupling and helical spin textures in 2D
heterostructure [Pb2BiS3][AuTe2]
SO SCIENTIFIC REPORTS
LA English
DT Article
ID TOPOLOGICAL INSULATORS; THIN-FILMS; WEAK-LOCALIZATION;
MAGNETORESISTANCE; BUCKHORNITE; SCATTERING; REGIME; TIME; HALL
AB Two-dimensional heterostructures with strong spin-orbit coupling have direct relevance to topological quantum materials and potential applications in spin-orbitronics. In this work, we report on novel quantum phenomena in [Pb2BiS3][AuTe2], a new 2D strong spin-orbit coupling heterostructure system. Transport measurements reveal the spin-related carrier scattering is at odds with the Abrikosov-Gorkov model due to strong spin-orbit coupling. This is consistent with our band structure calculations which reveal a large spin-orbit coupling gap of epsilon(so) = 0.21 eV. The band structure is also characterized by helical-like spin textures which are mainly induced by strong spin-orbit coupling and the inversion symmetry breaking in the heterostructure system.
C1 [Fang, L.; DeGottardi, W.; Glatz, A.; Matveev, K. A.; Kwok, W. -K.; Crabtree, G. W.; Kanatzidis, M. G.] Argonne Natl Lab, Div Mat Sci, 9700 S Cass Ave, Argonne, IL 60439 USA.
[Fang, L.; Kanatzidis, M. G.] Korea Res Inst Chem Technol, Adv Mat Div, Daejeon 305600, South Korea.
[Im, J.] Northwestern Univ, Dept Chem, 2145 Sheridan Rd, Evanston, IL 60208 USA.
[Jia, Y.] Northwestern Univ, NUFAB, Evanston, IL 60208 USA.
[Glatz, A.] Northern Illinois Univ, Dept Phys, De Kalb, IL 60115 USA.
RP DeGottardi, W; Kwok, WK; Kanatzidis, MG (reprint author), Argonne Natl Lab, Div Mat Sci, 9700 S Cass Ave, Argonne, IL 60439 USA.; Kanatzidis, MG (reprint author), Korea Res Inst Chem Technol, Adv Mat Div, Daejeon 305600, South Korea.
EM wdegottardi@anl.gov; wkwok@anl.gov; m-kanatzidis@northwestern.edu
FU US Department of Energy, Office of Science, Materials Sciences and
Engineering Division; Department of Energy, Office of Basic Energy
Sciences [DE-AC02-06CH11357]; Korea Research Institute of Chemical
Technology [KN1502-I00]
FX The authors are grateful to Ivar Martin, Vivek Mishra, Ulrich Welp and
Ralu Divan for useful discussions. Transport characterizations were
supported by the US Department of Energy, Office of Science, Materials
Sciences and Engineering Division. Synthesis and user facilities of the
Center for Nanoscale Materials were supported by the Department of
Energy, Office of Basic Energy Sciences, under Contract No.
DE-AC02-06CH11357. Theoretical calculations were supported by the Korea
Research Institute of Chemical Technology, under the project No.
KN1502-I00(JI).
NR 38
TC 0
Z9 0
U1 15
U2 15
PU NATURE PUBLISHING GROUP
PI LONDON
PA MACMILLAN BUILDING, 4 CRINAN ST, LONDON N1 9XW, ENGLAND
SN 2045-2322
J9 SCI REP-UK
JI Sci Rep
PD OCT 12
PY 2016
VL 6
AR 35313
DI 10.1038/srep35313
PG 7
WC Multidisciplinary Sciences
SC Science & Technology - Other Topics
GA DY3NX
UT WOS:000385002000002
PM 27731394
ER
PT J
AU Mota, A
Chen, Q
Foulk, JW
Ostien, JT
Lai, Z
AF Mota, A.
Chen, Q.
Foulk, J. W., III
Ostien, J. T.
Lai, Z.
TI A Cartesian parametrization for the numerical analysis of material
instability
SO INTERNATIONAL JOURNAL FOR NUMERICAL METHODS IN ENGINEERING
LA English
DT Article
DE material stability; constitutive equations; Newton methods; variational
methods
ID DISCONTINUOUS MATERIAL BIFURCATION; SOFTENING CONSTITUTIVE-EQUATIONS;
MODELING STRONG DISCONTINUITIES; FINITE-ELEMENT METHOD; VARIATIONAL
FORMULATION; STRAIN LOCALIZATION; MATERIAL STABILITY; SOLID MECHANICS;
PLASTICITY; FAILURE
AB We examine four parametrizations of the unit sphere in the context of material stability analysis by means of the singularity of the acoustic tensor. We then propose a Cartesian parametrization for vectors that lie a cube of side length two and use these vectors in lieu of unit normals to test for the loss of the ellipticity condition. This parametrization is then used to construct a tensor akin to the acoustic tensor. It is shown that both of these tensors become singular at the same time and in the same planes in the presence of a material instability. The performance of the Cartesian parametrization is compared against the other parametrizations, with the results of these comparisons showing that in general, the Cartesian parametrization is more robust and more numerically efficient than the others. Copyright (c) 2016 John Wiley & Sons, Ltd.
C1 [Mota, A.; Foulk, J. W., III; Ostien, J. T.] Sandia Natl Labs, Mech Mat Dept, Livermore, CA 94550 USA.
[Chen, Q.; Lai, Z.] Clemson Univ, Glenn Dept Civil Engn, Clemson, SC 29634 USA.
RP Chen, Q (reprint author), Clemson Univ, Glenn Dept Civil Engn, Clemson, SC 29634 USA.
EM qiushi@clemson.edu
FU US Department of Energy's (DOE) Advanced Simulation and Computing (ASC)
Program at Sandia National Laboratories; US Department of Energy's
National Nuclear Security Administration [DE-AC04-94AL85000]
FX Support for this work was received through the US Department of Energy's
(DOE) Advanced Simulation and Computing (ASC) Program at Sandia National
Laboratories. Sandia National Laboratories is a multiprogram laboratory
managed and operated by Sandia Corporation, a wholly owned subsidiary of
Lockheed Martin Corporation, for the US Department of Energy's National
Nuclear Security Administration under contract DE-AC04-94AL85000.
NR 41
TC 1
Z9 1
U1 3
U2 3
PU WILEY-BLACKWELL
PI HOBOKEN
PA 111 RIVER ST, HOBOKEN 07030-5774, NJ USA
SN 0029-5981
EI 1097-0207
J9 INT J NUMER METH ENG
JI Int. J. Numer. Methods Eng.
PD OCT 12
PY 2016
VL 108
IS 2
BP 156
EP 180
DI 10.1002/nme.5228
PG 25
WC Engineering, Multidisciplinary; Mathematics, Interdisciplinary
Applications
SC Engineering; Mathematics
GA DX1MW
UT WOS:000384132500004
ER
PT J
AU Trott, JF
Kim, J
Abu Aboud, O
Wettersten, H
Stewart, B
Berryhill, G
Uzal, F
Hovey, RC
Chen, CH
Anderson, K
Graef, A
Sarver, AL
Modiano, JF
Weiss, RH
AF Trott, Josephine F.
Kim, Jeffrey
Abu Aboud, Omran
Wettersten, Hiromi
Stewart, Benjamin
Berryhill, Grace
Uzal, Francisco
Hovey, Russell C.
Chen, Ching-Hsien
Anderson, Katie
Graef, Ashley
Sarver, Aaron L.
Modiano, Jaime F.
Weiss, Robert H.
TI Inhibiting tryptophan metabolism enhances interferon therapy in kidney
cancer
SO ONCOTARGET
LA English
DT Article
DE tryptophan; kynurenine; renal cell carcinoma; interferon-alpha;
indolamine-2,3-dioxygenase
ID RENAL-CELL CARCINOMA; INDOLEAMINE 2,3-DIOXYGENASE; METABOLOMICS
ANALYSIS; IMMUNE ESCAPE; ALPHA; GAMMA; GENE; CHEMOTHERAPY; DEGRADATION;
SUPPRESSION
AB Renal cell carcinoma (RCC) is increasing in incidence, and a complete cure remains elusive. While immune-checkpoint antibodies are promising, interferon-based immunotherapy has been disappointing. Tryptophan metabolism, which produces immunosuppressive metabolites, is enhanced in RCC. Here we show indolamine-2,3-dioxygenase- 1 (IDO1) expression, a kynurenine pathway enzyme, is increased not only in tumor cells but also in the microenvironment of human RCC compared to normal kidney tissues. Neither kynurenine metabolites nor IDO inhibitors affected the survival or proliferation of human RCC or murine renal cell adenocarcinoma (RENCA) cells in vitro. However, interferon-gamma (IFN gamma) induced high levels of IDO1 in both RCC and RENCA cells, concomitant with enhanced kynurenine levels in conditioned media. Induction of IDO1 by IFN alpha was weaker than by IFN gamma. Neither the IDO1 inhibitor methyl-thiohydantoin-DL-tryptophan (MTH-trp) nor IFNa alone inhibited RENCA tumor growth, however the combination of MTH-trp and IFNa reduced tumor growth compared to IFNa. Thus, the failure of IFNa therapy for human RCC is likely due to its inability to overcome the immunosuppressive environment created by increased IDO1. Based on our data, and given that IDO inhibitors are already in clinical trials for other malignancies, IFNa therapy with an IDO inhibitor should be revisited for RCC.
C1 [Trott, Josephine F.; Kim, Jeffrey; Abu Aboud, Omran; Wettersten, Hiromi; Chen, Ching-Hsien; Weiss, Robert H.] Univ Calif Davis, Div Nephrol, Sch Med, Davis, CA 95616 USA.
[Trott, Josephine F.; Berryhill, Grace; Hovey, Russell C.] Univ Calif Davis, Dept Anim Sci, Davis, CA 95616 USA.
[Weiss, Robert H.] Univ Calif Davis, Ctr Comprehens Canc, Davis, CA 95616 USA.
[Stewart, Benjamin] Lawrence Livermore Natl Lab, Biosci & Biotechnol Div, Livermore, CA USA.
[Uzal, Francisco] Univ Calif Davis, Sch Vet Med, Calif Anim Hlth & Food Safety Lab, San Bernardino, CA USA.
[Anderson, Katie; Graef, Ashley; Sarver, Aaron L.; Modiano, Jaime F.] Univ Minnesota, Coll Vet Med, Anim Canc Care & Res Program, St Paul, MN 55108 USA.
[Anderson, Katie; Graef, Ashley; Modiano, Jaime F.] Univ Minnesota, Coll Vet Med, Dept Vet Clin Sci, St Paul, MN 55108 USA.
[Anderson, Katie; Graef, Ashley; Sarver, Aaron L.; Modiano, Jaime F.] Mason Canc Ctr, Minneapolis, MN USA.
[Modiano, Jaime F.] Ctr Immunol, Minneapolis, MN USA.
[Modiano, Jaime F.] Univ Minnesota, Stem Cell Inst, Minneapolis, MN USA.
[Weiss, Robert H.] VA Northern Calif Hlth Care Syst, Med Serv, Sacramento, CA USA.
[Wettersten, Hiromi] Univ Calif San Diego, Sanford Consortium Regenerat Med, La Jolla, CA USA.
RP Weiss, RH (reprint author), Univ Calif Davis, Div Nephrol, Sch Med, Davis, CA 95616 USA.; Weiss, RH (reprint author), Univ Calif Davis, Ctr Comprehens Canc, Davis, CA 95616 USA.; Weiss, RH (reprint author), VA Northern Calif Hlth Care Syst, Med Serv, Sacramento, CA USA.
EM rhweiss@ucdavis.edu
FU NIH [1R03CA181837-01, 1R01DK082690-01A1]; Medical Service of the US
Department of Veterans Affairs; Dialysis Clinics, Inc. (DCI); LLNL-UC
Fitzpatrick Postdoctoral Award; NCI [F31 CA189421, F30 CA195973];
Academic Federation Research Grant Program Innovative Development Award;
Perlman Chair in Animal Oncology
FX This work was supported by NIH grants 1R03CA181837-01,
1R01DK082690-01A1, the Medical Service of the US Department of Veterans
Affairs, and Dialysis Clinics, Inc. (DCI) (R.H.W). H.I.W was supported
by the LLNL-UC Fitzpatrick Postdoctoral Award, G.E.B by the Ruth L.
Kirschstein Pre-doctoral National Research Service Award from NCI (F31
CA189421), K.L.A by the Ruth L. Kirschstein National Research Service
Award from NCI (F30 CA195973), J.F.T by the Academic Federation Research
Grant Program Innovative Development Award and J.F.M by the Perlman
Chair in Animal Oncology.
NR 38
TC 0
Z9 0
U1 7
U2 7
PU IMPACT JOURNALS LLC
PI ALBANY
PA 6211 TIPTON HOUSE, STE 6, ALBANY, NY 12203 USA
SN 1949-2553
J9 ONCOTARGET
JI Oncotarget
PD OCT 11
PY 2016
VL 7
IS 41
BP 66540
EP 66557
DI 10.18632/oncotarget.11658
PG 18
WC Oncology; Cell Biology
SC Oncology; Cell Biology
GA EB5UO
UT WOS:000387446200018
PM 27572319
ER
PT J
AU Hora, H
Korn, G
Eliezer, S
Nissim, N
Lalousis, P
Giuffrida, L
Margarone, D
Picciotto, A
Miley, GH
Moustaizis, S
Martinez-Val, JM
Barty, CPJ
Kirchhoff, GJ
AF Hora, H.
Korn, G.
Eliezer, S.
Nissim, N.
Lalousis, P.
Giuffrida, L.
Margarone, D.
Picciotto, A.
Miley, G. H.
Moustaizis, S.
Martinez-Val, J. -M.
Barty, C. P. J.
Kirchhoff, G. J.
TI Avalanche boron fusion by laser picosecond block ignition with magnetic
trapping for clean and economic reactor
SO HIGH POWER LASER SCIENCE AND ENGINEERING
LA English
DT Article
DE boron fusion energy; dielectric nonlinear force explosion; economic
reactor; environmentally clean energy; picosecond-non-thermal plasma
block ignition
ID DRIVEN PLASMA BLOCKS; PULSES; ENERGY; TARGETS; ACCELERATION;
COMPRESSION; INTENSITIES
AB Measured highly elevated gains of proton-boron (HB11) fusion (Picciotto et al., Phys. Rev. X 4, 031030 (2014)) confirmed the exceptional avalanche reaction process (Lalousis et al., Laser Part. Beams 32, 409 (2014); Hora et al., Laser Part. Beams 33, 607 (2015)) for the combination of the non-thermal block ignition using ultrahigh intensity laser pulses of picoseconds duration. The ultrahigh acceleration above 10(20) cm s(-2) for plasma blocks was theoretically and numerically predicted since 1978 (Hora, Physics of Laser Driven Plasmas (Wiley, 1981), pp. 178 and 179) and measured (Sauerbrey, Phys. Plasmas 3, 4712 (1996)) in exact agreement (Hora et al., Phys. Plasmas 14, 072701 (2007)) when the dominating force was overcoming thermal processes. This is based on Maxwell's stress tensor by the dielectric properties of plasma leading to the nonlinear (ponderomotive) force f(NL) resulting in ultra-fast expanding plasma blocks by a dielectric explosion. Combining this with measured ultrahigh magnetic fields and the avalanche process opens an option for an environmentally absolute clean and economic boron fusion power reactor. This is supported also by other experiments with very high HB11 reactions under different conditions (Labaune et al., Nature Commun. 4, 2506 (2013)).
C1 [Hora, H.] Univ New South Wales, Dept Theoret Phys, Sydney, NSW 2052, Australia.
[Korn, G.; Giuffrida, L.; Margarone, D.] PALS Ctr, Inst Phys, ELI Beamline Project, ASCR, Prague, Czech Republic.
[Eliezer, S.; Martinez-Val, J. -M.] Univ Politecn Madrid, Inst Nucl Fus, Madrid, Spain.
[Eliezer, S.; Nissim, N.] Soreq Res Ctr, Yavne, Israel.
[Lalousis, P.] Inst Elect Struct & Lasers FORTH, Iraklion, Greece.
[Picciotto, A.] Fdn Bruno Kessler, Micronano Facil, I-38123 Trento, Italy.
[Miley, G. H.] Univ Illinois, Dept Nucl Plasma & Radiol Engn, Urbana, IL 61801 USA.
[Moustaizis, S.] Tech Univ Crete, Lab Matter Struct & Laser Phys, Khania, Greece.
[Barty, C. P. J.] Lawrence Livermore Natl Lab, Livermore, CA USA.
[Kirchhoff, G. J.] UJK Management GmbH, D-85586 Poing, Germany.
RP Hora, H (reprint author), Univ New South Wales, Dept Theoret Phys, Sydney, NSW 2052, Australia.
EM h.hora@unsw.edu.au
NR 66
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U1 2
U2 2
PU CAMBRIDGE UNIV PRESS
PI CAMBRIDGE
PA EDINBURGH BLDG, SHAFTESBURY RD, CB2 8RU CAMBRIDGE, ENGLAND
SN 2095-4719
EI 2052-3289
J9 HIGH POWER LASER SCI
JI High Power Laser Sci. Eng.
PD OCT 11
PY 2016
VL 4
AR e35
DI 10.1017/hpl.2016.29
PG 9
WC Optics
SC Optics
GA DZ8EH
UT WOS:000386102800001
ER
PT J
AU Sun, C
Taguchi, AT
Vermaas, JV
Beal, NJ
O'Malley, PJ
Tajkliorshid, E
Gennis, RB
Dikanov, SA
AF Sun, Chang
Taguchi, Alexander T.
Vermaas, Josh V.
Beal, Nathan J.
O'Malley, Patrick J.
Tajkliorshid, Emad
Gennis, Robert B.
Dikanov, Sergei A.
TI Q-Band Electron-Nuclear Double Resonance Reveals Out-of-Plane Hydrogen
Bonds Stabilize an Anionic Ubisemiquinone in Cytochrome bo(3) from
Escherichia coli
SO BIOCHEMISTRY
LA English
DT Article
ID QUINONE-BINDING-SITE; PHOTOSYNTHETIC REACTION CENTERS; GUI
MEMBRANE-BUILDER; PARTICLE MESH EWALD; UBIQUINOL OXIDASE; Q(H) SITE;
PARAMAGNETIC-RESONANCE; MOLECULAR-DYNAMICS; Q(H)(CENTER-DOT-)
UBISEMIQUINONE; BOUND UBIQUINONE
AB The respiratory cytochrome bo(3) ubiquinol oxidase from Escherichia coli has a high-affinity ubiquinone binding site that stabilizes the one-electron reduced ubisemiquinone (SQ(H)), which is a transient intermediate during the electron-mediated reduction of O-2 to water. It is known that SQ(H) is stabilized by two strong hydrogen bonds from R71 and D75 to ubiquinone carbonyl oxygen O1 and weak hydrogen bonds from H98 and Q101 to O4. In this work, SQ(H) was investigated with orientation-selective Q-band (similar to 34 GHz) pulsed H-1 electron-nuclear double resonance (ENDOR) spectroscopy on fully deuterated cytochrome (cyt) bo(3) in a H2O solvent so that only exchangeable protons contribute to the observed ENDOR spectra. Simulations of the experimental ENDOR spectra provided the principal values and directions of the hyperfine (hfi) tensors for the two strongly coupled H-bond protons (H1 and H2). For H1, the largest principal component of the proton anisotropic hfi tensor T-z' = 11.8 MHz, whereas for H2, T-z' = 8.6 MHz. Remarkably, the data show that the direction of the H1 H-bond is nearly perpendicular to the quinone plane (similar to 70 degrees out of plane). The orientation of the second strong hydrogen bond, H2, is out of plane by similar to 25 degrees. Equilibrium molecular dynamics simulations on a membrane-embedded model of the cyt bo(3) Q(H) site show that these H-bond orientations are plausible but do not distinguish which H-bond, from R71 or D75, is nearly perpendicular to the quinone ring. Density functional theory calculations support the idea that the distances and geometries of the H-bonds to the ubiquinone carbonyl oxygens, along with the measured proton anisotropic hfi couplings, are most compatible with an anionic (deprotonated) ubisemiquinone.
C1 [Sun, Chang; Vermaas, Josh V.; Tajkliorshid, Emad; Gennis, Robert B.] Univ Illinois, Dept Biochem, Urbana, IL 61801 USA.
[Taguchi, Alexander T.; Vermaas, Josh V.; Tajkliorshid, Emad; Gennis, Robert B.] Univ Illinois, Ctr Biophys & Computat Biol, Urbana, IL 61801 USA.
[Taguchi, Alexander T.; Dikanov, Sergei A.] Univ Illinois, Dept Vet Clin Med, Urbana, IL 61801 USA.
[Tajkliorshid, Emad] Univ Illinois, Beckman Inst, Urbana, IL 61801 USA.
[Beal, Nathan J.; O'Malley, Patrick J.] Univ Manchester, Sch Chem, Manchester M13 9PL, Lancs, England.
[Taguchi, Alexander T.] MIT, Dept Chem, Cambridge, MA 02139 USA.
[Vermaas, Josh V.] Natl Renewable Energy Lab, Biosci Ctr, Golden, CO 80401 USA.
RP Tajkliorshid, E; Gennis, RB (reprint author), Univ Illinois, Dept Biochem, Urbana, IL 61801 USA.; Tajkliorshid, E; Gennis, RB (reprint author), Univ Illinois, Ctr Biophys & Computat Biol, Urbana, IL 61801 USA.; Dikanov, SA (reprint author), Univ Illinois, Dept Vet Clin Med, Urbana, IL 61801 USA.; Tajkliorshid, E (reprint author), Univ Illinois, Beckman Inst, Urbana, IL 61801 USA.; O'Malley, PJ (reprint author), Univ Manchester, Sch Chem, Manchester M13 9PL, Lancs, England.
EM patrick.omalley@manchester.ac.uk; emad@life.illinois.edu;
r-gennis@illinois.edu; dikanov@illinois.edu
OI Sun, Chang/0000-0001-6070-5545
FU Chemical Sciences, Geosciences and Biosciences Division, Office of Basic
Energy Sciences, Office of Sciences, U.S. Department of Energy
[DE-FG02-08ER15960, DE-FG02-87ER13716]; National Center for Research
Resources [S10-RR15878, S10-RR025438]; National Institutes of Health
(NIH) [U54-GM087519, P41-RR05969]; Office of Science of the U.S.
Department of Energy [DE-ACO2-05CH11231]; Molecular Biophysics Training
Program [5T32-GM008276]; Sandia National Laboratories Campus Executive
Program - Laboratory Directed Research and Development (LDRD) Program at
Sandia National Laboratories; U.S. Department of Energy's National
Nuclear Security Administration [DE-AC04-94AL85000]
FX This research was supported by Grants DE-FG02-08ER15960 (S.A.D.) and
DE-FG02-87ER13716 (R.B.G.) from the Chemical Sciences, Geosciences and
Biosciences Division, Office of Basic Energy Sciences, Office of
Sciences, U.S. Department of Energy, and National Center for Research
Resources Grants S10-RR15878 and S10-RR025438 for pulsed EPR
instrumentation. The computational work at the University of Illinois at
Urbana-Champaign was supported by grants from the National Institutes of
Health (NIH) to E.T. (U54-GM087519 and P41-RR05969), using resources of
the National Energy Research Scientific Computing Center, a DOE Office
of Science User Facility supported by the Office of Science of the U.S.
Department of Energy under Contract No. DE-ACO2-05CH11231. P.J.O.
acknowledges the use of computer resources granted by the EPSRC UK
national service for computational chemistry software (NSCCS). A.T.T.
and J.V.V. gratefully acknowledge past support as NIH trainees of the
Molecular Biophysics Training Program (5T32-GM008276). J.V.V. also
acknowledges support from the Sandia National Laboratories Campus
Executive Program, which is funded by the Laboratory Directed Research
and Development (LDRD) Program at Sandia National Laboratories. Sandia
is a multiprogram laboratory managed and operated by Sandia Corp., a
wholly owned subsidiary of Lockheed Martin Corp., for the U.S.
Department of Energy's National Nuclear Security Administration under
Contract DE-AC04-94AL85000.
NR 66
TC 0
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U1 3
U2 3
PU AMER CHEMICAL SOC
PI WASHINGTON
PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA
SN 0006-2960
J9 BIOCHEMISTRY-US
JI Biochemistry
PD OCT 11
PY 2016
VL 55
IS 40
BP 5714
EP 5725
DI 10.1021/acs.biochem.6b00669
PG 12
WC Biochemistry & Molecular Biology
SC Biochemistry & Molecular Biology
GA DY7VA
UT WOS:000385336200007
PM 27622672
ER
PT J
AU Liu, J
Huq, A
Moorhead-Rosenberg, Z
Manthiram, A
Page, K
AF Liu, Jue
Huq, Ashfia
Moorhead-Rosenberg, Zachary
Manthiram, Arumugam
Page, Katharine
TI Nanoscale Ni/Mn Ordering in the High Voltage Spinel Cathode
LiNi0.5Mn1.5O4
SO CHEMISTRY OF MATERIALS
LA English
DT Article
ID LITHIUM-ION BATTERIES; PAIR DISTRIBUTION FUNCTION; LIXNI0.5MN1.5O4;
INTERCALATION; LINIXMN2-XO4; IMPACT
C1 [Liu, Jue; Huq, Ashfia; Page, Katharine] Oak Ridge Natl Lab, Chem & Engn Mat Div, Oak Ridge, TN 37831 USA.
[Moorhead-Rosenberg, Zachary; Manthiram, Arumugam] Univ Texas Austin, Mat Sci & Engn Program, Austin, TX 78712 USA.
[Moorhead-Rosenberg, Zachary; Manthiram, Arumugam] Univ Texas Austin, Texas Mat Inst, Austin, TX 78712 USA.
RP Page, K (reprint author), Oak Ridge Natl Lab, Chem & Engn Mat Div, Oak Ridge, TN 37831 USA.
EM pagekl@ornl.gov
RI Page, Katharine/C-9726-2009; Huq, Ashfia/J-8772-2013
OI Page, Katharine/0000-0002-9071-3383; Huq, Ashfia/0000-0002-8445-9649
FU U.S. Department of Energy, Office of Science, Office of Basic Energy
Sciences, Early Career Research Program [KC040602, DE-AC05-00OR22725];
Scientific User Facilities Division, Office of Basic Sciences, U.S.
Department of Energy; U.S. Department of Energy, Office of Basic Energy
Sciences, Division of Materials Sciences and Engineering [DE-SC0005397]
FX Work by J.L. and K.P. was supported through the U.S. Department of
Energy, Office of Science, Office of Basic Energy Sciences, Early Career
Research Program award KC040602, under contract number
DE-AC05-00OR22725. Research conducted at POWGEN beamline at ORNL's
Spallation Neutron Source was sponsored by the Scientific User
Facilities Division, Office of Basic Sciences, U.S. Department of
Energy. The sample synthesis work at the University of Texas at Austin
was supported by the U.S. Department of Energy, Office of Basic Energy
Sciences, Division of Materials Sciences and Engineering under award
number DE-SC0005397.
NR 28
TC 0
Z9 0
U1 29
U2 29
PU AMER CHEMICAL SOC
PI WASHINGTON
PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA
SN 0897-4756
EI 1520-5002
J9 CHEM MATER
JI Chem. Mat.
PD OCT 11
PY 2016
VL 28
IS 19
BP 6817
EP 6821
DI 10.1021/acs.chemmater.6b02946
PG 5
WC Chemistry, Physical; Materials Science, Multidisciplinary
SC Chemistry; Materials Science
GA DY7VD
UT WOS:000385336500003
ER
PT J
AU Rosales, BA
Men, L
Cady, SD
Hanrahan, MP
Rossini, AJ
Vela, J
AF Rosales, Bryan A.
Men, Long
Cady, Sarah D.
Hanrahan, Michael P.
Rossini, Aaron J.
Vela, Javier
TI Persistent Dopants and Phase Segregation in Organolead Mixed-Halide
Perovskites
SO CHEMISTRY OF MATERIALS
LA English
DT Article
ID ORGANOMETAL TRIHALIDE PEROVSKITE; NUCLEAR-MAGNETIC-RESONANCE; PB-207
NMR-SPECTROSCOPY; LIGHT-EMITTING-DIODES; HYBRID SOLAR-CELLS;
OPTICAL-PROPERTIES; LEAD HALIDES; SPINODAL DECOMPOSITION; CH3NH3PBX3 X;
ELECTRONIC-STRUCTURE
AB Organolead mixed-halide perovskites such as CH3NH3PbX3-aXa' (X, X' = I, Br, Cl) are interesting semiconductors because of their low cost, high photovoltaic power conversion efficiencies, enhanced moisture stability, and band gap tunability. Using a combination of optical absorption spectroscopy, powder X-ray diffraction (XRD), and, for the first time, Pb-207 solid state nuclear magnetic resonance (ssNMR), we probe the extent of alloying and phase segregation in these materials. Because Pb-207 ssNMR chemical shifts are highly sensitive to local coordination and electronic structure, and vary linearly with halogen electronegativity and band gap, this technique can provide the true chemical speciation and composition of organolead mixed-halide perovskites. We specifically investigate samples made by three different preparative methods: solution phase synthesis, thermal annealing, and solid phase synthesis. Pb-207 ssNMR reveals that nonstoichiometric dopants and semicrystalline phases are prevalent in samples made by solution phase synthesis. We show that these nanodomains are persistent after thermal annealing up to 200 degrees C. Further, a novel solid phase synthesis that starts from the parent, single-halide perovskites can suppress phase segregation but not the formation of dopants. Our observations are consistent with the presence of miscibility gaps and spontaneous spinodal decomposition of the mixed-halide perovskites at room temperature. This underscores how strongly different synthetic procedures impact the nanostructuring and composition of organolead halide perovskites. Better optoelectronic properties and improved device stability and performance may be achieved through careful manipulation of the different phases and nanodomains present in these materials.
C1 [Rosales, Bryan A.; Men, Long; Cady, Sarah D.; Hanrahan, Michael P.; Rossini, Aaron J.; Vela, Javier] Iowa State Univ, Dept Chem, Ames, IA 50011 USA.
[Cady, Sarah D.] Iowa State Univ, Chem Instrumentat Facil, Ames, IA 50011 USA.
[Men, Long; Hanrahan, Michael P.; Rossini, Aaron J.; Vela, Javier] US DOE, Ames Lab, Ames, IA 50011 USA.
RP Vela, J (reprint author), Iowa State Univ, Dept Chem, Ames, IA 50011 USA.; Vela, J (reprint author), US DOE, Ames Lab, Ames, IA 50011 USA.
EM vela@iastate.edu
RI Vela, Javier/I-4724-2014
OI Vela, Javier/0000-0001-5124-6893
FU U.S. Department of Energy, Office of Basic Energy Sciences, Division of
Chemical Sciences, Geosciences, and Biosciences through the Ames
Laboratory; U.S. Department of Energy [DE-AC02-07CH11358]; Ames
Laboratory Royalty Account; Iowa State University
FX This research is supported by the U.S. Department of Energy, Office of
Basic Energy Sciences, Division of Chemical Sciences, Geosciences, and
Biosciences through the Ames Laboratory. The Ames Laboratory is operated
for the U.S. Department of Energy by Iowa State University under
Contract No. DE-AC02-07CH11358. We thank K.-J. Galayda and R. S. Houk at
Ames Laboratory for ICP-MS assistance. A.J.R. thanks the Ames Laboratory
Royalty Account and Iowa State University for funding.
NR 92
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U1 29
U2 29
PU AMER CHEMICAL SOC
PI WASHINGTON
PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA
SN 0897-4756
EI 1520-5002
J9 CHEM MATER
JI Chem. Mat.
PD OCT 11
PY 2016
VL 28
IS 19
BP 6848
EP 6859
DI 10.1021/acs.chemmater.6b01874
PG 12
WC Chemistry, Physical; Materials Science, Multidisciplinary
SC Chemistry; Materials Science
GA DY7VD
UT WOS:000385336500007
ER
PT J
AU Wan, LWF
Incorvati, JT
Poeppelmeier, KR
Prendergast, D
AF Wan, Liwen F.
Incorvati, Jared T.
Poeppelmeier, Kenneth R.
Prendergast, David
TI Building a Fast Lane for Mg Diffusion in alpha-MoO3 by Fluorine Doping
SO CHEMISTRY OF MATERIALS
LA English
DT Article
ID AUGMENTED-WAVE METHOD; CATHODE MATERIALS; INTERCALATION; MOLYBDENUM;
BATTERIES; LITHIUM; METALS
AB Following previous experimental work examining a layered oxyfluoride as cathode material for Mg-ion batteries [Incorvati et al., Chem. Mater. 2016, 28, 17], we study the role of fluorination on the structural and electronic properties of molybdenum trioxide and its impact on Mg intercalation and diffusion using first principles methods. Although bulk alpha-MoO3 is a 2D layered compound, we find that it provides 3D channels for Mg diffusion. When F atoms are incorporated into the alpha-MoO3 lattice, they replace the O atoms sitting at a specific crystallographic site that is linked by two nearest Mo atoms within a single Mo-O layer. As a consequence of F substitution, the local Mo-anion bonds are distorted, which leads to closure of the electronic band gap. From the analysis of zone center phonon vibrational frequencies, it is found that the local Mo-anion bonding strength is weakened by replacing O2- with F-, which ultimately facilitates Mg diffusion through the F-substituted lattice. For example, it is shown that upon fluorination the activation barriers for Mg diffusion along selected pathways can be lowered by as much as 0.6 eV, estimated from our nudged elastic band simulations at 0K. Our results imply that direct anion doping can be a viable approach toward improving ion diffusivity in Mg-ion battery cathodes.
C1 [Wan, Liwen F.; Incorvati, Jared T.; Poeppelmeier, Kenneth R.; Prendergast, David] Argonne Natl Lab, Joint Ctr Energy Storage Res, 9700 S Cass Ave, Argonne, IL 60439 USA.
[Wan, Liwen F.; Prendergast, David] Lawrence Berkeley Natl Lab, Mol Foundry, Berkeley, CA 94720 USA.
[Incorvati, Jared T.; Poeppelmeier, Kenneth R.] Northwestern Univ, Dept Chem, 2145 Sheridan Rd, Evanston, IL 60208 USA.
RP Wan, LWF (reprint author), Argonne Natl Lab, Joint Ctr Energy Storage Res, 9700 S Cass Ave, Argonne, IL 60439 USA.; Wan, LWF (reprint author), Lawrence Berkeley Natl Lab, Mol Foundry, Berkeley, CA 94720 USA.
EM LWan@lbl.gov
FU Joint Center for Energy Storage Research, an Energy Innovation Hub -
U.S. Department of Energy, Office of Science, Basic Energy Sciences;
Office of Science of the U.S. Department of Energy [DE-AC02-05CH11231]
FX We acknowledge Dr. J. T. Vaughey for very helpful discussions. This work
was supported by the Joint Center for Energy Storage Research, an Energy
Innovation Hub funded by the U.S. Department of Energy, Office of
Science, Basic Energy Sciences. The computations were supported by a
User Project at The Molecular Foundry using the computing cluster
(vulcan), managed by the High Performance Computing Services Group, at
Lawrence Berkeley National Laboratory (LBNL) and the resources of the
National Energy Research Scientific Computing Center, LBNL, both of
which are supported by the Office of Science of the U.S. Department of
Energy under contract No. DE-AC02-05CH11231.
NR 21
TC 1
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U1 24
U2 24
PU AMER CHEMICAL SOC
PI WASHINGTON
PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA
SN 0897-4756
EI 1520-5002
J9 CHEM MATER
JI Chem. Mat.
PD OCT 11
PY 2016
VL 28
IS 19
BP 6900
EP 6908
DI 10.1021/acs.chemmater.6b02223
PG 9
WC Chemistry, Physical; Materials Science, Multidisciplinary
SC Chemistry; Materials Science
GA DY7VD
UT WOS:000385336500013
ER
PT J
AU Stavrou, E
Lobanov, S
Dong, HF
Oganov, AR
Prakapenka, VB
Konopkova, Z
Goncharov, AF
AF Stavrou, Elissaios
Lobanov, Sergey
Dong, Huafeng
Oganov, Artem R.
Prakapenka, Vitali B.
Konopkova, Zuzana
Goncharov, Alexander F.
TI Synthesis of Ultra-incompressible spa-Hybridized Carbon Nitride with 1:1
Stoichiometry
SO CHEMISTRY OF MATERIALS
LA English
DT Article
ID SHOCK COMPRESSION; CRYSTAL-STRUCTURE; HIGH-PRESSURES; PHASE-DIAGRAM;
DIAMOND; C3N4; TEMPERATURES; PREDICTION; SILICON; SYSTEM
AB The search of compounds with CxNy composition holds great promise for creating materials which would rival diamond in hardness due to the very strong covalent C-N bond. Early theoretical and experimental works on CxNy compounds were based on the hypothetical structural similarity of predicted C3N4 phases with known binary A(3)B(4) structural types; however, the synthesis of C3N4 other than g-C3N4 remains elusive. Here, we explore an elemental synthesis at high pressures and temperatures in which the compositional limitations due to the use of precursors in the early works are substantially lifted. Using in situ synchrotron X-ray diffraction and Raman spectroscopy, we demonstrate the synthesis of a highly incompressible Pnnm CN compound (x = y = 1) with sp(3)-hybridized carbon above 55 GPa and 7000 K. This result is supported by first-principles evolutionary search, which finds that CN is the most stable compound above 14 GPa. On pressure release below 6 GPa, the synthesized CN compound amorphizes, maintaining its 1:1 stoichiometry as confirmed by energy-dispersive X-ray spectroscopy. This work underscores the importance of understanding the novel high-pressure chemistry laws that promote extended 3D C-N structures, never observed at ambient conditions. Moreover, it opens a new route for synthesis of superhard materials based on novel stoichiometries
C1 [Stavrou, Elissaios; Lobanov, Sergey; Goncharov, Alexander F.] Carnegie Inst Sci, Geophys Lab, Washington, DC 20015 USA.
[Stavrou, Elissaios; Goncharov, Alexander F.] Lawrence Livermore Natl Lab, Phys & Life Sci Directorate, POB 808,L-350, Livermore, CA 94550 USA.
[Lobanov, Sergey] Russian Acad Sci, Siberian Branch, Sobolev Inst Geol & Mineral, 3 Pr Ac Koptyga, Novosibirsk 630090, Russia.
[Dong, Huafeng; Oganov, Artem R.] SUNY Stony Brook, Inst Adv Computat Sci, Ctr Mat Design, Dept Geosci, Stony Brook, NY 11794 USA.
[Oganov, Artem R.] Skolkovo Innovat Ctr, Skolkovo Inst Sci & Technol, 5 Nobel St, Moscow 143026, Russia.
[Oganov, Artem R.] Moscow Inst Phys & Technol, 9 Inst Skiy Lane, Dolgoprudny City 141700, Moscow Region, Russia.
[Oganov, Artem R.] Northwestern Polytech Univ, Sch Mat Sci, Xian 710072, Peoples R China.
[Prakapenka, Vitali B.] Univ Chicago, Ctr Adv Radiat Sources, Chicago, IL 60637 USA.
[Konopkova, Zuzana] DESY Photon Sci, D-22607 Hamburg, Germany.
[Goncharov, Alexander F.] Univ Sci & Technol China, Hefei 230026, Peoples R China.
[Goncharov, Alexander F.] Chinese Acad Sci, Inst Solid State Phys, Key Lab Mat Phys, Hefei 230031, Peoples R China.
[Goncharov, Alexander F.] Chinese Acad Sci, Inst Solid State Phys, Ctr Energy Matter Extreme Environm, Hefei 230031, Peoples R China.
RP Stavrou, E; Goncharov, AF (reprint author), Carnegie Inst Sci, Geophys Lab, Washington, DC 20015 USA.; Stavrou, E; Goncharov, AF (reprint author), Lawrence Livermore Natl Lab, Phys & Life Sci Directorate, POB 808,L-350, Livermore, CA 94550 USA.; Goncharov, AF (reprint author), Univ Sci & Technol China, Hefei 230026, Peoples R China.; Goncharov, AF (reprint author), Chinese Acad Sci, Inst Solid State Phys, Key Lab Mat Phys, Hefei 230031, Peoples R China.; Goncharov, AF (reprint author), Chinese Acad Sci, Inst Solid State Phys, Ctr Energy Matter Extreme Environm, Hefei 230031, Peoples R China.
EM stavrou1@llnl.gov; agoncharov@carnegiescience.edu
RI Lobanov, Sergey/D-9405-2017
OI Lobanov, Sergey/0000-0001-9728-2363
FU DARPA [W31P4Q1210008]; National Natural Science Foundation of China
[21473211]; Deep Carbon Observatory DCO; Chinese Academy of Sciences
[2011T2J20]; Recruitment Program of Foreign Experts; Ministry of
Education and Science of Russian Federation [14.B25.31.0032]; U.S.
Department of Energy by Lawrence Livermore National Security, LLC
[DE-AC-52-07NA27344]; U.S. NSF [EAR-0622171, DMR-1231586]; DOE
Geosciences [DE-FG02-94ER14466]; DOE-BES [DE-AC02-06CH11357]; European
Community [312284]; [0330-2014-0013]
FX E.S. thanks Karl Syassen for providing high quality natural graphite.
S.L. thanks John Armstrong for technical assistance with SEM. This work
was supported by the DARPA (grant No. W31P4Q1210008), the National
Natural Science Foundation of China (Grant no. 21473211), and the Deep
Carbon Observatory DCO. A.F.G. was partly supported by the Chinese
Academy of Sciences visiting professorship for senior international
scientists (Grant No. 2011T2J20) and Recruitment Program of Foreign
Experts. S.L. was partly supported by the Ministry of Education and
Science of Russian Federation (No. 14.B25.31.0032) and by state
assignment project No. 0330-2014-0013. Part of this work was performed
under the auspices of the U.S. Department of Energy by Lawrence
Livermore National Security, LLC, under Contract DE-AC-52-07NA27344.
GSECARS is supported by the U.S. NSF (EAR-0622171, DMR-1231586) and DOE
Geosciences (DE-FG02-94ER14466). Use of the APS was supported by the
DOE-BES under Contract No. DE-AC02-06CH11357. The research leading to
these results has received funding from the European Community's Seventh
Framework Programme (FP7/2007-2013) under grant agreement no. 312284.
Portions of this research were carried out at the light source PETRA III
at DESY, a member of the Helmholtz Association (HGF).
NR 51
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PU AMER CHEMICAL SOC
PI WASHINGTON
PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA
SN 0897-4756
EI 1520-5002
J9 CHEM MATER
JI Chem. Mat.
PD OCT 11
PY 2016
VL 28
IS 19
BP 6925
EP 6933
DI 10.1021/acs.chemmater.6b02593
PG 9
WC Chemistry, Physical; Materials Science, Multidisciplinary
SC Chemistry; Materials Science
GA DY7VD
UT WOS:000385336500016
ER
PT J
AU Li, T
Karwal, S
Aoun, B
Zhao, HY
Ren, Y
Canlas, CP
Elam, JW
Winans, RE
AF Li, Tao
Karwal, Saurabh
Aoun, Bachir
Zhao, Haiyan
Ren, Yang
Canlas, Christian P.
Elam, Jeffrey W.
Winans, Randall E.
TI Exploring Pore Formation of Atomic Layer-Deposited Overlayers by in Situ
Small- and Wide-Angle X-ray Scattering
SO CHEMISTRY OF MATERIALS
LA English
DT Article
ID COPPER CHROMITE CATALYSTS; SELECTIVE HYDROGENATION; PHASE REACTIONS;
STABILITY; NANOPARTICLES; VIRUS; FILMS; TIO2
AB In this work, we explore the pore structure of overcoated materials by in situ synchrotron small-angle (SAXS) and wide-angle X-ray scattering (WAXS). Thin films of aluminum oxide (Al2O3) and titanium dioxide (TiO2) with thicknesses of 4.9 and 2.5 nm, respectively, are prepared by atomic layer deposition (ALD) on nonporous nanoparticles. In situ X-ray measurements reveal that porosity is induced in the ALD films by annealing the samples at high temperatures. Moreover, this pore formation can be attributed to densification resulting from an amorphous to crystalline phase transition of the ALD films as confirmed by high-resolution X-ray diffraction and the pair distribution function. Simultaneous SAXS and WAXS results show not only that the porosity is formed by the phase transition but also that the pore size increases with temperature.
C1 [Li, Tao; Aoun, Bachir; Zhao, Haiyan; Ren, Yang; Winans, Randall E.] Argonne Natl Lab, Xray Sci Div, 9700 S Cass Ave, Argonne, IL 60439 USA.
[Karwal, Saurabh; Canlas, Christian P.; Elam, Jeffrey W.] Argonne Natl Lab, Div Energy Syst, 9700 S Cass Ave, Argonne, IL 60439 USA.
[Zhao, Haiyan] Univ Idaho, Chem & Mat Engn Dept, Idaho Falls, ID 83401 USA.
RP Winans, RE (reprint author), Argonne Natl Lab, Xray Sci Div, 9700 S Cass Ave, Argonne, IL 60439 USA.
EM rewinans@anl.gov
FU Institute for Atom-efficient Chemical Transformations (IACT), an Energy
Frontier Research Center - U.S. Department of Energy, Office of Basic
Energy Sciences; U.S. DOE [DE-AC02-06CH11357]
FX This material is based upon work supported as part of the Institute for
Atom-efficient Chemical Transformations (IACT), an Energy Frontier
Research Center funded by the U.S. Department of Energy, Office of Basic
Energy Sciences. The authors acknowledge the use of the Advanced Photon
Source, an Office of Science User Facility operated for the U.S.
Department of Energy (DOE) Office of Science by Argonne National
Laboratory, was supported by the U.S. DOE under Contract
DE-AC02-06CH11357.
NR 28
TC 1
Z9 1
U1 13
U2 13
PU AMER CHEMICAL SOC
PI WASHINGTON
PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA
SN 0897-4756
EI 1520-5002
J9 CHEM MATER
JI Chem. Mat.
PD OCT 11
PY 2016
VL 28
IS 19
BP 7082
EP 7087
DI 10.1021/acs.chemmater.6b03222
PG 6
WC Chemistry, Physical; Materials Science, Multidisciplinary
SC Chemistry; Materials Science
GA DY7VD
UT WOS:000385336500033
ER
PT J
AU Guo, XF
Szenknect, S
Mesbah, A
Clavier, N
Poinssot, C
Wu, D
Xu, HW
Dacheux, N
Ewing, RC
Navrotsky, A
AF Guo, Xiaofeng
Szenknect, Stephanie
Mesbah, Adel
Clavier, Nicolas
Poinssot, Christophe
Wu, Di
Xu, Hongwu
Dacheux, Nicolas
Ewing, Rodney C.
Navrotsky, Alexandra
TI Energetics of a Uranothorite (Th1-xUxSiO4) Solid Solution
SO CHEMISTRY OF MATERIALS
LA English
DT Article
ID HIGH-TEMPERATURE CALORIMETRY; NATURAL FISSION REACTORS; THORITE MINERAL
GROUP; CIGAR LAKE DEPOSIT; METASOMATIZED GRANITE; ISOTOPIC ANALYSES;
NUCLEAR-FUEL; WASTE FORMS; X-RAY; COFFINITE
AB High-temperature oxide melt solution calorimetric measurements were completed to determine the enthalpies of formation of the uranothorite, (USiO4)(x)-(ThSiO4)(1-x), solid solution. Phase-pure samples with x values of 0, 0.11, 0.21, 0.35, 0.71, and 0.84 were prepared, purified, and characterized by powder X-ray diffraction, electron probe microanalysis, thermogravimetric analysis and differential scanning calorimetry coupled with in situ mass spectrometry, and high temperature oxide melt solution calorimetry. This work confirms the energetic metastability of coffinite, USiO4, and U-rich intermediate silicate phases with respect to a mixture of binary oxides. However, variations in unit cell parameters and negative excess volumes of mixing, coupled with strongly exothermic enthalpies of mixing in the solid solution, suggest short-range cation ordering that can stabilize intermediate compositions, especially near x = 0.5.
C1 [Guo, Xiaofeng; Xu, Hongwu] Los Alamos Natl Lab, Earth & Environm Sci Div, Los Alamos, NM 87545 USA.
[Guo, Xiaofeng; Navrotsky, Alexandra] Univ Calif Davis, Peter A Rock Thermochem Lab, Davis, CA 95616 USA.
[Guo, Xiaofeng; Navrotsky, Alexandra] Univ Calif Davis, NEAT ORU, Davis, CA 95616 USA.
[Szenknect, Stephanie; Mesbah, Adel; Clavier, Nicolas; Dacheux, Nicolas] Univ Montpellier, ENSCM, Inst Chim Separat Marcoule, ICSM UMR 5257,CNRS CEA, Site Marcoule Bat 426,BP 17171, F-30207 Bagnols Sur Ceze, France.
[Poinssot, Christophe] CEA, Nucl Energy Div, Radiochem & Proc Dept, BP 17171, F-30207 Bagnols Sur Ceze, France.
[Wu, Di] Washington State Univ, Gene & Linda Voiland Sch Chem Engn & Bioengn, Pullman, WA 99163 USA.
[Ewing, Rodney C.] Stanford Univ, Dept Geol Sci, Stanford, CA 94305 USA.
RP Navrotsky, A (reprint author), Univ Calif Davis, Peter A Rock Thermochem Lab, Davis, CA 95616 USA.; Navrotsky, A (reprint author), Univ Calif Davis, NEAT ORU, Davis, CA 95616 USA.
EM anavrotsky@ucdavis.edu
RI Wu, Di/A-3039-2014; mesbah, adel/A-4559-2011;
OI Wu, Di/0000-0001-6879-321X; mesbah, adel/0000-0002-6905-2402; Xu,
Hongwu/0000-0002-0793-6923
FU U.S. Department of Energy (DOE), Office of Science, Office of Basic
Energy Sciences [DE-SC0001089]; Laboratory Directed Research and
Development (LDRD) program, through the G. T. Seaborg Institute, of Los
Alamos National Laboratory (LANL) under DOE; NEEDS Resources program of
the CNRS (French National Center for Scientific Research)
[DE-AC52-06NA25396]
FX Calorimetric measurements at the University of California at Davis and
later analyses of data were supported by the Materials Science of
Actinides, an Energy Frontier Research Center, funded by the U.S.
Department of Energy (DOE), Office of Science, Office of Basic Energy
Sciences, under Grant DE-SC0001089. X.G. was also supported by a Seaborg
postdoctoral fellowship from the Laboratory Directed Research and
Development (LDRD) program, through the G. T. Seaborg Institute, of Los
Alamos National Laboratory (LANL), which is operated by Los Alamos
National Security LLC, under DOE Contract DE-AC52-06NA25396. The
experiments associated with the preparation and characterization of
single-phase and homogeneous uranothorite solid solutions were supported
by the NEEDS Resources program of the CNRS (French National Center for
Scientific Research).
NR 64
TC 0
Z9 0
U1 11
U2 11
PU AMER CHEMICAL SOC
PI WASHINGTON
PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA
SN 0897-4756
EI 1520-5002
J9 CHEM MATER
JI Chem. Mat.
PD OCT 11
PY 2016
VL 28
IS 19
BP 7117
EP 7124
DI 10.1021/acs.chemmater.6b03346
PG 8
WC Chemistry, Physical; Materials Science, Multidisciplinary
SC Chemistry; Materials Science
GA DY7VD
UT WOS:000385336500037
ER
PT J
AU Predota, M
Machesky, ML
Wesolowski, DJ
AF Predota, Milan
Machesky, Michael L.
Wesolowski, David J.
TI Molecular Origins of the Zeta Potential
SO LANGMUIR
LA English
DT Article
ID ELECTRIC DOUBLE-LAYER; RUTILE 110 SURFACE; HIGH-IONIC-STRENGTH; ZERO
CHARGE; DYNAMICS SIMULATION; INTERFACIAL WATER; HYDRATION WATER;
NANOPARTICLES; ADSORPTION; SILICA
AB The zeta potential (ZP) is an oft-reported measure of the macroscopic charge state of solid surfaces and colloidal particles in contact with solvents. However, the origin of this readily measurable parameter has remained divorced from the molecular-level processes governing the underlying electrokinetic phenomena, which limits its usefulness. Here, we connect the macroscopic measure to the microscopic realm through nonequilibrium molecular dynamics simulations of electroosmotic flow between parallel slabs of the hydroxylated (110) rutile (TiO2) surface. These simulations provided streaming mobilities, which were converted to ZP via the commonly used Helmholtz-Smoluchowski equation. A range of rutile surface charge densities (0.1 to -0.4 C/m(2)), corresponding to pH values between about 2.8 and 9.4, in RbCl, NaCl, and SrCl2 aqueous solutions, were modeled and compared to experimental ZPs for TiO2 particle suspensions. Simulated ZPs qualitatively agree with experiment and show that anomalous ZP values and inequalities between the point of zero charge derived from electrokinetic versus pH titration measurements both arise from differing co- and counterion sorption affinities. We show that at the molecular level the ZP arises from the delicate interplay of spatially varying dynamics, structure, and electrostatics in a narrow interfacial region within about 15 angstrom of the surface, even in dilute salt solutions. This contrasts fundamentally with continuum descriptions of such interfaces, which predict the ZP response region to be inversely related to ionic strength. In reality the properties of this interfacial region are dominated by relatively immobile and structured water. Consequently, viscosity values are substantially greater than in the bulk, and electrostatic potential profiles are oscillatory in nature.
C1 [Predota, Milan] Univ South Bohemia, Fac Sci, Inst Phys & Biophys, Branisovska 1760, Ceske Budejovice 37005, Czech Republic.
[Machesky, Michael L.] Univ Illinois, Illinois State Water Survey, 2204 Griffith Dr, Champaign, IL 61820 USA.
[Wesolowski, David J.] Oak Ridge Natl Lab, Div Chem Sci, Oak Ridge, TN 37831 USA.
RP Predota, M (reprint author), Univ South Bohemia, Fac Sci, Inst Phys & Biophys, Branisovska 1760, Ceske Budejovice 37005, Czech Republic.
EM predota@prf.jcu.cz
RI Predota, Milan/A-2256-2009
OI Predota, Milan/0000-0003-3902-0992
FU Czech Science Foundation [13-08651S]; programme Center CERIT Scientific
Cloud, part of the Operational Program Research and Development for
Innovations [CZ. 1.05/3.2.00/08.0144]; U.S. Department of Energy, Office
of Science, Office of Basic Energy Sciences, Chemical Sciences,
Geosciences and Biosciences Division
FX M.P. was supported by the Czech Science Foundation Project 13-08651S.
Access to the CERIT-SC computing and storage facilities provided under
the programme Center CERIT Scientific Cloud, part of the Operational
Program Research and Development for Innovations, reg. no. CZ.
1.05/3.2.00/08.0144, is greatly appreciated. M.L.M. and D.J.W. were
supported by the U.S. Department of Energy, Office of Science, Office of
Basic Energy Sciences, Chemical Sciences, Geosciences and Biosciences
Division.
NR 63
TC 0
Z9 0
U1 30
U2 30
PU AMER CHEMICAL SOC
PI WASHINGTON
PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA
SN 0743-7463
J9 LANGMUIR
JI Langmuir
PD OCT 11
PY 2016
VL 32
IS 40
BP 10189
EP 10198
DI 10.1021/acs.langmuir.6b02493
PG 10
WC Chemistry, Multidisciplinary; Chemistry, Physical; Materials Science,
Multidisciplinary
SC Chemistry; Materials Science
GA DY7UY
UT WOS:000385336000006
PM 27643625
ER
PT J
AU Sun, L
Akgun, B
Narayanan, S
Jiang, Z
Foster, MD
AF Sun, Liang
Akgun, Bulent
Narayanan, Suresh
Jiang, Zhang
Foster, Mark D.
TI Surface Fluctuations of Polymer Brushes Swollen in Good Solvent Vapor
SO MACROMOLECULES
LA English
DT Article
ID RADICAL POLYMERIZATION; SILICA PARTICLES; WAVES; METHACRYLATE; DYNAMICS;
STYRENE
AB Swollen polymer brushes are found in various applications including biomedical coatings where the brush provides stability against harsh environmental conditions and mediates interactions with the surroundings. The surface height fluctuations of planar polystyrene brushes (0.04-0.61 chains/nm(2)) highly swollen in toluene vapor are so strongly slowed by the tethering of the chains that they are unobservable in the current experimental window of length and time. This is the case despite the fact that the segmental dynamics of the brush chains should be very fast due to the substantial plasticization by the solvent. With respect to thermally stimulated fluctuations, the surfaces of these swollen brushes are solidlike on time scales and length scales pertinent to many practical applications.
C1 [Sun, Liang; Foster, Mark D.] Univ Akron, Dept Polymer Sci, Akron, OH 44325 USA.
[Akgun, Bulent] NIST, NIST Ctr Neutron Res, Gaithersburg, MD 20899 USA.
[Akgun, Bulent] Univ Maryland, Dept Mat Sci & Engn, College Pk, MD 20742 USA.
[Akgun, Bulent] Bogazici Univ, Dept Chem, Istanbul, Turkey.
[Narayanan, Suresh; Jiang, Zhang] Argonne Natl Lab, Xray Sci Div, 9700 S Cass Ave, Argonne, IL 60439 USA.
RP Foster, MD (reprint author), Univ Akron, Dept Polymer Sci, Akron, OH 44325 USA.
EM mdf1@uakron.edu
RI Akgun, Bulent/H-3798-2011
FU DOE Office of Science by Argonne National Laboratory
[DE-AC02-06CH11357]; Bogazici University [B.U. 9080]
FX This research used resources of the Advanced Photon Source, a U.S.
Department of Energy (DOE) Office of Science User Facility operated for
the DOE Office of Science by Argonne National Laboratory under Contract
DE-AC02-06CH11357. B.A. acknowledges partial support by the Bogazici
University Research Fund (B.U. 9080).
NR 30
TC 0
Z9 0
U1 3
U2 3
PU AMER CHEMICAL SOC
PI WASHINGTON
PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA
SN 0024-9297
EI 1520-5835
J9 MACROMOLECULES
JI Macromolecules
PD OCT 11
PY 2016
VL 49
IS 19
BP 7308
EP 7313
DI 10.1021/acs.macromol.6b01081
PG 6
WC Polymer Science
SC Polymer Science
GA DY7UW
UT WOS:000385335800020
ER
PT J
AU Terban, MW
Dabbous, R
Debellis, AD
Poselt, E
Billinge, SJL
AF Terban, Maxwell W.
Dabbous, Raphael
Debellis, Anthony D.
Poeselt, Elmar
Billinge, Simon J. L.
TI Structures of Hard Phases in Thermoplastic Polyurethanes
SO MACROMOLECULES
LA English
DT Article
ID PAIR DISTRIBUTION FUNCTION; X-RAY-DIFFRACTION; AMORPHOUS POLYANILINE;
MICRODOMAIN STRUCTURE; CRYSTAL-STRUCTURE; BLOCK-COPOLYMERS; MODEL
COMPOUNDS; MDI UNITS; ELASTOMERS; SEGMENT
AB Limited long-range ordering and the presence of both hard and soft segments can cause substantial difficulties for structure determination in urethane elastomers. Here, the structuring has been investigated for a series of thermoplastic polyurethanes composed of 4,4'-methylene diphenyl diisocyanate and 1,4-butanediol. We utilize pair distribution function analysis of X-ray total scattering measurements to directly access the local structure and quantify the degree of ordering, showing that the structure varies significantly over the range of different component ratios investigated. A simple method is demonstrated for evaluating the viability of various structure candidates for the hard segment. The nature of the molecular conformations and packing is verified, allowing both ordered and disordered components to be quantified through structural modeling.
C1 [Terban, Maxwell W.; Billinge, Simon J. L.] Columbia Univ, Dept Appl Phys & Appl Math, New York, NY 10027 USA.
[Dabbous, Raphael] BASF Schweiz AG, CH-4058 Basel, Switzerland.
[Debellis, Anthony D.] BASF Corp, Quantum Chem & Hybrid Modeling Res, Tarrytown, NY 10591 USA.
[Poeselt, Elmar] BASF Polyurethanes GmbH, D-49448 Lemforde, Germany.
[Billinge, Simon J. L.] Brookhaven Natl Lab, Condensed Matter Phys & Mat Sci Dept, Upton, NY 11973 USA.
RP Billinge, SJL (reprint author), Columbia Univ, Dept Appl Phys & Appl Math, New York, NY 10027 USA.; Billinge, SJL (reprint author), Brookhaven Natl Lab, Condensed Matter Phys & Mat Sci Dept, Upton, NY 11973 USA.
EM sb2896@columbia.edu
FU DOE Office of Science [DE-AC02-98CH10886]; NSF [DMR-1534910]
FX This research used beamline X17A of the National Synchrotron Light
Source, a U.S. Department of Energy (DOE) Office of Science User
Facility operated for the DOE Office of Science by Brookhaven National
Laboratory under Contract DE-AC02-98CH10886. Support for S.J.L.B. was
funded by NSF through grant DMR-1534910.
NR 47
TC 1
Z9 1
U1 16
U2 16
PU AMER CHEMICAL SOC
PI WASHINGTON
PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA
SN 0024-9297
EI 1520-5835
J9 MACROMOLECULES
JI Macromolecules
PD OCT 11
PY 2016
VL 49
IS 19
BP 7350
EP 7358
DI 10.1021/acs.macromol.6b00889
PG 9
WC Polymer Science
SC Polymer Science
GA DY7UW
UT WOS:000385335800025
ER
PT J
AU Vakhshouri, K
Smith, BH
Chan, EP
Wang, CC
Salleo, A
Wang, C
Hexemer, A
Gomez, ED
AF Vakhshouri, Kiarash
Smith, Brandon H.
Chan, Edwin P.
Wang, Chenchen
Salleo, Alberto
Wang, Cheng
Hexemer, Alexander
Gomez, Enrique D.
TI Signatures of Intracrystallite and Intercrystallite Limitations of
Charge Transport in Polythiophenes
SO MACROMOLECULES
LA English
DT Article
ID FIELD-EFFECT TRANSISTORS; THIN-FILM TRANSISTORS; X-RAY-SCATTERING;
REGIOREGULAR POLY(3-HEXYL-THIOPHENE) DIODES; WEIGHT-DEPENDENT
MOBILITIES; SOLAR-CELL PERFORMANCE; CONJUGATED POLYMERS;
MOLECULAR-WEIGHT; SEMICRYSTALLINE POLYMERS; INTERCHAIN INTERACTIONS
AB Charge carrier mobilities in conjugated semicrystalline polymers depend on morphological parameters such as crystallinity, crystal orientation, and connectivity between ordered regions. Despite recent progress in the development of conducting polymers, the complex interplay between the aforementioned parameters and their impact on charge transport is not fully understood. By varying the casting solvents and thermal annealing, we have systematically modulated the crystallization of poly(3-hexylthiophene-2,5-diyl) (P3HT) and poly[2,5-bis(3-hexadecylthiophen-2-yl)thieno(3,2-b)thiophene] (PBTTT) thin films to examine the role of microstructure on charge mobilities. In particular, we achieve equal crystallinities through different processing routes to examine the role of structural parameters beyond the crystallinity on charge mobilities. As expected, a universal relationship does not exist between the crystallinity in either P3HT and PBTTT active layers and the charge mobility in devices. In P3HT films, higher boiling point solvents yield longer conjugation lengths, an indicator of stronger intracrystalline order, and therefore higher device mobilities. In contrast, the charge mobilities of PBTTT devices depend on the interconnectivity between crystallites and intercrystalline order in the active layer.
C1 [Vakhshouri, Kiarash; Smith, Brandon H.; Gomez, Enrique D.] Penn State Univ, Dept Chem Engn, University Pk, PA 16802 USA.
[Gomez, Enrique D.] Penn State Univ, Mat Res Inst, University Pk, PA 16802 USA.
[Chan, Edwin P.] NIST, Div Polymers, Gaithersburg, MD 20899 USA.
[Wang, Chenchen; Salleo, Alberto] Stanford Univ, Mat Sci & Engn, Stanford, CA 94305 USA.
[Wang, Cheng; Hexemer, Alexander] Lawrence Berkeley Natl Lab, Adv Light Source, Berkeley, CA 94530 USA.
RP Gomez, ED (reprint author), Penn State Univ, Dept Chem Engn, University Pk, PA 16802 USA.; Gomez, ED (reprint author), Penn State Univ, Mat Res Inst, University Pk, PA 16802 USA.
EM edg12@psu.edu
RI Wang, Cheng/A-9815-2014
FU Center for Flexible Electronics at Penn State - Dow Chemical Company;
NSF [DMR-1056199]; Advanced Light Source, Lawrence Berkeley National
Laboratory; U.S. Department of Energy [DE-AC02-05CH11231]
FX Duc T. Duong is gratefully acknowledged for assistance in analyzing
absorption spectra. Major funding for this work was provided by the
Center for Flexible Electronics at Penn State sponsored by The Dow
Chemical Company and NSF under Grant DMR-1056199. The authors also
acknowledge the support of the Advanced Light Source, Lawrence Berkeley
National Laboratory, which is supported by the U.S. Department of Energy
under Contract DE-AC02-05CH11231.
NR 97
TC 0
Z9 0
U1 24
U2 24
PU AMER CHEMICAL SOC
PI WASHINGTON
PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA
SN 0024-9297
EI 1520-5835
J9 MACROMOLECULES
JI Macromolecules
PD OCT 11
PY 2016
VL 49
IS 19
BP 7359
EP 7369
DI 10.1021/acs.macromol.6b01086
PG 11
WC Polymer Science
SC Polymer Science
GA DY7UW
UT WOS:000385335800026
ER
PT J
AU Bisogni, V
Catalano, S
Green, RJ
Gibert, M
Scherwitzl, R
Huang, YB
Strocov, VN
Zubko, P
Balandeh, S
Triscone, JM
Sawatzky, G
Schmitt, T
AF Bisogni, Valentina
Catalano, Sara
Green, Robert J.
Gibert, Marta
Scherwitzl, Raoul
Huang, Yaobo
Strocov, Vladimir N.
Zubko, Pavlo
Balandeh, Shadi
Triscone, Jean-Marc
Sawatzky, George
Schmitt, Thorsten
TI Ground-state oxygen holes and the metal-insulator transition in the
negative charge-transfer rare-earth nickelates
SO NATURE COMMUNICATIONS
LA English
DT Article
ID X-RAY-SCATTERING; ELECTRONIC-STRUCTURE; ABSORPTION SPECTROSCOPY; RNIO3
PEROVSKITES; NDNIO3 FILMS; BAND-GAP; EXCITATIONS; SPIN; ND
AB The metal-insulator transition and the intriguing physical properties of rare-earth perovskite nickelates have attracted considerable attention in recent years. Nonetheless, a complete understanding of these materials remains elusive. Here we combine X-ray absorption and resonant inelastic X-ray scattering (RIXS) spectroscopies to resolve important aspects of the complex electronic structure of rare-earth nickelates, taking NdNiO3 thin film as representative example. The unusual coexistence of bound and continuum excitations observed in the RIXS spectra provides strong evidence for abundant oxygen holes in the ground state of these materials. Using cluster calculations and Anderson impurity model interpretation, we show that distinct spectral signatures arise from a Ni 3d(8) configuration along with holes in the oxygen 2p valence band, confirming suggestions that these materials do not obey a conventional positive charge-transfer picture, but instead exhibit a negative charge-transfer energy in line with recent models interpreting the metal-insulator transition in terms of bond disproportionation.
C1 [Bisogni, Valentina; Huang, Yaobo; Strocov, Vladimir N.; Schmitt, Thorsten] Paul Scherrer Inst, Res Dept Synchrotron Radiat & Nanotechnol, CH-5232 Villigen, Switzerland.
[Bisogni, Valentina] Brookhaven Natl Lab, Natl Synchrotron Light Source 2, Upton, NY 11973 USA.
[Catalano, Sara; Gibert, Marta; Scherwitzl, Raoul; Zubko, Pavlo; Triscone, Jean-Marc] Univ Geneva, Dept Quantum Matter Phys, 24 Quai Ernest Ansermet, CH-1211 Geneva 4, Switzerland.
[Green, Robert J.; Balandeh, Shadi; Sawatzky, George] Univ British Columbia, Dept Phys & Astron, Vancouver, BC V6T 1Z1, Canada.
[Green, Robert J.; Sawatzky, George] Univ British Columbia, Quantum Matter Inst, Vancouver, BC V6T 1Z4, Canada.
[Huang, Yaobo] Chinese Acad Sci, Beijing Natl Lab Condensed Matter Phys, Beijing 100190, Peoples R China.
[Huang, Yaobo] Chinese Acad Sci, Inst Phys, Beijing 100190, Peoples R China.
[Zubko, Pavlo] UCL, London Ctr Nanotechnol, 17-19 Gordon St, London WC1H 0HA, England.
[Zubko, Pavlo] UCL, Dept Phys & Astron, 17-19 Gordon St, London WC1H 0HA, England.
RP Bisogni, V; Schmitt, T (reprint author), Paul Scherrer Inst, Res Dept Synchrotron Radiat & Nanotechnol, CH-5232 Villigen, Switzerland.; Bisogni, V (reprint author), Brookhaven Natl Lab, Natl Synchrotron Light Source 2, Upton, NY 11973 USA.
EM bisogni@bnl.gov; thorsten.schmitt@psi.ch
RI Zubko, Pavlo/B-5496-2009; Gibert, Marta/A-2317-2016; Schmitt,
Thorsten/A-7025-2010
OI Zubko, Pavlo/0000-0002-7330-3163; Gibert, Marta/0000-0001-8856-6831;
FU Swiss National Science Foundation through its National Centre of
Competence in Research MaNEP; Sinergia network Mott Physics Beyond the
Heisenberg (MPBH) model; European Community's Seventh Framework Program
(FP7) [290605]; ERC Grant [319286]; Canadian funding agency NSERC;
Canadian funding agency CRC; Max Planck/UBC center for Quantum Materials
FX This work was performed at the ADRESS beamline of the Swiss Light Source
at the Paul Scherrer Institut, Switzerland. Part of this research has
been funded by the Swiss National Science Foundation through its
National Centre of Competence in Research MaNEP and the Sinergia network
Mott Physics Beyond the Heisenberg (MPBH) model. The research leading to
these results has received funding from the European Community's Seventh
Framework Program (FP7/2007-2013) under Grant Agreement No. 290605
(COFUND: PSI-FELLOW) and ERC Grant Agreement No. 319286 (Q-MAC).
Moreover, this work has received support through funding from the
Canadian funding agencies NSERC, CRC, and the Max Planck/UBC center for
Quantum Materials.
NR 54
TC 1
Z9 1
U1 38
U2 38
PU NATURE PUBLISHING GROUP
PI LONDON
PA MACMILLAN BUILDING, 4 CRINAN ST, LONDON N1 9XW, ENGLAND
SN 2041-1723
J9 NAT COMMUN
JI Nat. Commun.
PD OCT 11
PY 2016
VL 7
AR 13017
DI 10.1038/ncomms13017
PG 8
WC Multidisciplinary Sciences
SC Science & Technology - Other Topics
GA DZ0SS
UT WOS:000385550600001
PM 27725665
ER
PT J
AU Eshet, H
Baer, R
Neuhauser, D
Rabani, E
AF Eshet, Hagai
Baer, Roi
Neuhauser, Daniel
Rabani, Eran
TI Theory of highly efficient multiexciton generation in type-II nanorods
SO NATURE COMMUNICATIONS
LA English
DT Article
ID MULTIPLE EXCITON GENERATION; SEMICONDUCTOR QUANTUM DOTS; CARBON NANOTUBE
PHOTODIODES; CARRIER MULTIPLICATION; SOLAR-CELLS; 1ST-PRINCIPLES
CALCULATIONS; COLLOIDAL NANOSTRUCTURES; AUGER RECOMBINATION; SEEDED
NANORODS; SINGLE-PHOTON
AB Multiexciton generation, by which more than a single electron-hole pair is generated on optical excitation, is a promising paradigm for pushing the efficiency of solar cells beyond the Shockley-Queisser limit of 31%. Utilizing this paradigm, however, requires the onset energy of multiexciton generation to be close to twice the band gap energy and the efficiency to increase rapidly above this onset. This challenge remains unattainable even using confined nanocrystals, nanorods or nanowires. Here, we show how both goals can be achieved in a nanorod heterostructure with type-II band offsets. Using pseudopotential atomistic calculation on a model type-II semiconductor heterostructure we predict the optimal conditions for controlling multiexciton generation efficiencies at twice the band gap energy. For a finite band offset, this requires a sharp interface along with a reduction of the exciton cooling and may enable a route for breaking the Shockley-Queisser limit.
C1 [Eshet, Hagai] Tel Aviv Univ, Sackler Fac Exact Sci, Sch Chem, IL-69978 Tel Aviv, Israel.
[Eshet, Hagai; Rabani, Eran] Tel Aviv Univ, Raymond & Beverly Sackler Ctr Computat Mol & Mat, IL-69978 Tel Aviv, Israel.
[Baer, Roi] Hebrew Univ Jerusalem, Inst Chem, Fritz Haber Ctr Mol Dynam, IL-91904 Jerusalem, Israel.
[Neuhauser, Daniel] Univ Calif Los Angeles, Dept Chem, Los Angeles, CA 90024 USA.
[Rabani, Eran] Univ Calif Berkeley, Dept Chem, Berkeley, CA 94720 USA.
[Rabani, Eran] Lawrence Berkeley Natl Lab, Div Mat Sci, Berkeley, CA 94720 USA.
RP Rabani, E (reprint author), Tel Aviv Univ, Raymond & Beverly Sackler Ctr Computat Mol & Mat, IL-69978 Tel Aviv, Israel.; Baer, R (reprint author), Hebrew Univ Jerusalem, Inst Chem, Fritz Haber Ctr Mol Dynam, IL-91904 Jerusalem, Israel.; Neuhauser, D (reprint author), Univ Calif Los Angeles, Dept Chem, Los Angeles, CA 90024 USA.; Rabani, E (reprint author), Univ Calif Berkeley, Dept Chem, Berkeley, CA 94720 USA.; Rabani, E (reprint author), Lawrence Berkeley Natl Lab, Div Mat Sci, Berkeley, CA 94720 USA.
EM roi.baer@huji.ac.il; dxn@chem.ucla.edu; eran.rabani@berkeley.edu
FU Pitzer Center; Kavli Institute of the University of California,
Berkeley; ISF [189/14]; NSF [CHE-1465064, CHE-1112500]
FX R.B. gratefully acknowledges support for his sabbatical visit by the
Pitzer Center and the Kavli Institute of the University of California,
Berkeley and the ISF grant 189/14. E.R. and D.N. acknowledge support
from NSF grants CHE-1465064 and CHE-1112500, respectively.
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PI LONDON
PA MACMILLAN BUILDING, 4 CRINAN ST, LONDON N1 9XW, ENGLAND
SN 2041-1723
J9 NAT COMMUN
JI Nat. Commun.
PD OCT 11
PY 2016
VL 7
AR 13178
DI 10.1038/ncomms13178
PG 6
WC Multidisciplinary Sciences
SC Science & Technology - Other Topics
GA DZ0QS
UT WOS:000385545400001
PM 27725668
ER
PT J
AU Olefeldt, D
Goswami, S
Grosse, G
Hayes, D
Hugelius, G
Kuhry, P
McGuire, AD
Romanovsky, VE
Sannel, ABK
Schuur, EAG
Turetsky, MR
AF Olefeldt, D.
Goswami, S.
Grosse, G.
Hayes, D.
Hugelius, G.
Kuhry, P.
McGuire, A. D.
Romanovsky, V. E.
Sannel, A. B. K.
Schuur, E. A. G.
Turetsky, M. R.
TI Circumpolar distribution and carbon storage of thermokarst landscapes
SO NATURE COMMUNICATIONS
LA English
DT Article
ID PERMAFROST CARBON; THAWING PERMAFROST; CLIMATE; FEEDBACK; FORESTS;
ALASKA; PEATLANDS; DYNAMICS; DATABASE; RELEASE
AB Thermokarst is the process whereby the thawing of ice- rich permafrost ground causes land subsidence, resulting in development of distinctive landforms. Accelerated thermokarst due to climate change will damage infrastructure, but also impact hydrology, ecology and biogeochemistry. Here, we present a circumpolar assessment of the distribution of thermokarst landscapes, defined as landscapes comprised of current thermokarst landforms and areas susceptible to future thermokarst development. At 3.6 x 10(6) km(2), thermokarst landscapes are estimated to cover similar to 20% of the northern permafrost region, with approximately equal contributions from three landscape types where characteristic wetland, lake and hillslope thermokarst landforms occur. We estimate that approximately half of the below-ground organic carbon within the study region is stored in thermokarst landscapes. Our results highlight the importance of explicitly considering thermokarst when assessing impacts of climate change, including future landscape greenhouse gas emissions, and provide a means for assessing such impacts at the circumpolar scale.
C1 [Olefeldt, D.] Univ Alberta, Dept Renewable Resources, Edmonton, AB T6G 2H1, Canada.
[Olefeldt, D.; Turetsky, M. R.] Univ Guelph, Dept Integrat Biol, Guelph, ON N1G 2W1, Canada.
[Goswami, S.] Oak Ridge Natl Lab, Div Environm Sci, Oak Ridge, TN 37831 USA.
[Goswami, S.] Indian Space Res Org, Natl Remote Sensing Ctr, Hyderabad 500037, Andhra Pradesh, India.
[Grosse, G.] Helmholtz Ctr Polar & Marine Res, Alfred Wegener Inst, Telegrafenberg A45, D-14473 Potsdam, Germany.
[Hayes, D.] Univ Maine, Sch Forest Resources, Orono, ME 04473 USA.
[Hugelius, G.; Kuhry, P.; Sannel, A. B. K.] Stockholm Univ, Dept Phys Geog, S-10691 Stockholm, Sweden.
[McGuire, A. D.] Univ Alaska, Alaska Cooperat Fish & Wildlife Res Unit, US Geol Survey, Fairbanks, AK 99775 USA.
[Romanovsky, V. E.] Univ Alaska, Inst Geophys, Fairbanks, AK 99775 USA.
[Romanovsky, V. E.] Tyumen State Oil & Gas Univ, Tyumen 625000, Tyument Oblast, Russia.
[Schuur, E. A. G.] No Arizona Univ, Ctr Ecosyst Sci & Soc, Flagstaff, AZ 86011 USA.
RP Olefeldt, D (reprint author), Univ Alberta, Dept Renewable Resources, Edmonton, AB T6G 2H1, Canada.; Olefeldt, D (reprint author), Univ Guelph, Dept Integrat Biol, Guelph, ON N1G 2W1, Canada.
EM olefeldt@ualberta.ca
RI Olefeldt, David/E-8835-2013; Grosse, Guido/F-5018-2011
OI Olefeldt, David/0000-0002-5976-1475; Grosse, Guido/0000-0001-5895-2141
FU National Science Foundation Network Grant [955713]; National Science
Foundation SEARCH Grant [1331083]; Campus Alberta Innovates Program; ERC
[338335]; HGF [ERC-0013]; Department of Energy (DOE) [3ERKP818]; Swedish
Research Council; EU JPI COUP consortium; U.S. Geological Survey Alaska
Climate Science Center; U.S. Geological Survey Land Carbon Program; U.S.
Department of Energy Office of Science, Office of Biological and
Environmental Sciences Division Terrestrial Ecosystem Sciences program
[DE-SC0006982]
FX This project benefited from input from members of the Permafrost Carbon
Network (www.permafrostcarbon.org). Supporting funding to the Permafrost
Carbon Network was provided by the National Science Foundation Network
Grant #955713 and the National Science Foundation SEARCH Grant #1331083.
Author contributions were also supported by individual grants: D.O.-the
Campus Alberta Innovates Program, G.G.-ERC #338335 and HGF #ERC-0013,
D.H.-Department of Energy (DOE) Early Career Award (DOEBER #3ERKP818),
G.H.-the Swedish Research Council and the EU JPI COUP consortium,
A.D.M.-the U.S. Geological Survey Alaska Climate Science Center and the
U.S. Geological Survey Land Carbon Program, E.A.G.S-U.S. Department of
Energy Office of Science, Office of Biological and Environmental
Sciences Division Terrestrial Ecosystem Sciences program, Award
#DE-SC0006982. Thanks goes to Andrew Balser, Benjamin Abbott, Claire
Treat and Cristian Estop-Aragones for carrying out evaluations of the
thermokarst landscape maps. Guangsheng Chen aided the climate data
analysis and Andrew Kohlenberg created the figures, helped design the
expert evaluation and expanded the database of study sites. Any use of
trade, firm or product names is for descriptive purposes only and does
not imply endorsement by the U.S. Government.
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PA MACMILLAN BUILDING, 4 CRINAN ST, LONDON N1 9XW, ENGLAND
SN 2041-1723
J9 NAT COMMUN
JI Nat. Commun.
PD OCT 11
PY 2016
VL 7
AR 13043
DI 10.1038/ncomms13043
PG 11
WC Multidisciplinary Sciences
SC Science & Technology - Other Topics
GA DZ0QO
UT WOS:000385545000001
PM 27725633
ER
PT J
AU Chen, HJ
Narayan, A
Fang, L
Calta, NP
Shi, FY
Chung, DY
Wagner, LK
Kwok, WK
Kanatzidis, MG
AF Chen, Haijie
Narayan, Awadhesh
Fang, Lei
Calta, Nicholas P.
Shi, Fengyuan
Chung, Duck Young
Wagner, Lucas K.
Kwok, Wai-Kwong
Kanatzidis, Mercouri G.
TI From complex magnetism ordering to simple ferromagnetism in
two-dimensional LaCrSb3 by hole doping
SO PHYSICAL REVIEW B
LA English
DT Article
ID CHARGE-DENSITY-WAVE; SQUARE NETS; 43 K; SUPERCONDUCTIVITY;
MAGNETORESISTANCE; TELLURIUM; YBRH2SI2; BEHAVIOR; SYSTEM; CU
AB Competing orders widely exist in many material systems, such as superconductivity, magnetism, and ferroelectricity; LaCrSb3 is a highly anisotropic magnetic material in which the spins are aligned ferromagnetically in one direction and canted antiferromagnetically in another in the Cr-Sb chains. Hole doping with Sr2+ and Ca2+ in the La site suppresses the antiferromagnetic correlations and transforms the anisotropic magnetic order into a ferromagnetic lattice in all directions. First-principles density functional theory calculations show that the canted magnetic order becomes energetically less favorable compared to the FM order upon hole doping. Doping in the La site is an effective approach to modulate the competing orders in LaCrSb3.
C1 [Chen, Haijie; Fang, Lei; Calta, Nicholas P.; Kanatzidis, Mercouri G.] Northwestern Univ, Dept Chem, 2145 Sheridan Rd, Evanston, IL 60208 USA.
[Shi, Fengyuan; Kanatzidis, Mercouri G.] Northwestern Univ, Dept Mat Sci & Engn, Evanston, IL 60208 USA.
[Chen, Haijie; Fang, Lei; Chung, Duck Young; Kwok, Wai-Kwong; Kanatzidis, Mercouri G.] Argonne Natl Lab, Div Mat Sci, 9700 S Cass Ave, Argonne, IL 60439 USA.
[Narayan, Awadhesh; Wagner, Lucas K.] Univ Illinois, Dept Phys, Urbana, IL 61801 USA.
RP Kanatzidis, MG (reprint author), Northwestern Univ, Dept Chem, 2145 Sheridan Rd, Evanston, IL 60208 USA.; Kanatzidis, MG (reprint author), Northwestern Univ, Dept Mat Sci & Engn, Evanston, IL 60208 USA.; Kanatzidis, MG (reprint author), Argonne Natl Lab, Div Mat Sci, 9700 S Cass Ave, Argonne, IL 60439 USA.
EM m-kanatzidis@northwestern.edu
FU Center for Emergent Superconductivity, an Energy Frontier Research
Center - U.S. Department of Energy, Office of Science, Office of Basic
Energy Sciences [DEAC0298CH1088]; Soft and Hybrid Nanotechnology
Experimental (SHyNE) Resource (NSF) [NNCI-1542205]; Materials Research
Science and Engineering Center (MRSEC) program (NSF) at the Materials
Research Center [DMR-1121262]; International Institute for
Nanotechnology (IIN); Keck Foundation; State of Illinois through the IIN
FX This paper was supported by the Center for Emergent Superconductivity,
an Energy Frontier Research Center funded by the U.S. Department of
Energy, Office of Science, Office of Basic Energy Sciences, under Award
No. DEAC0298CH1088. Computational resources were provided by the
University of Illinois Campus Cluster. We made use of the Electron Probe
Instrumentation Center (EPIC) facility of the Northwestern University
Atomic and Nanoscale Characterization Experimental Center (NUANCE)
Center at Northwestern University, which has received support from the
Soft and Hybrid Nanotechnology Experimental (SHyNE) Resource (NSF
NNCI-1542205), the Materials Research Science and Engineering Center
(MRSEC) program (NSF DMR-1121262) at the Materials Research Center, the
International Institute for Nanotechnology (IIN), the Keck Foundation,
and the State of Illinois through the IIN.
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PI COLLEGE PK
PA ONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA
SN 2469-9950
EI 2469-9969
J9 PHYS REV B
JI Phys. Rev. B
PD OCT 11
PY 2016
VL 94
IS 13
AR 134411
DI 10.1103/PhysRevB.94.134411
PG 6
WC Physics, Condensed Matter
SC Physics
GA DZ1SL
UT WOS:000385619900002
ER
PT J
AU Kissikov, T
Dioguardi, AP
Timmons, EI
Tanatar, MA
Prozorov, R
Bud'ko, SL
Canfield, PC
Fernandes, RM
Curro, NJ
AF Kissikov, T.
Dioguardi, A. P.
Timmons, E. I.
Tanatar, M. A.
Prozorov, R.
Bud'ko, S. L.
Canfield, P. C.
Fernandes, R. M.
Curro, N. J.
TI NMR study of nematic spin fluctuations in a detwinned single crystal of
underdoped Ba(Fe1-xCox)(2)As2
SO PHYSICAL REVIEW B
LA English
DT Article
ID IRON-BASED SUPERCONDUCTORS; ARSENIDE SUPERCONDUCTOR; DENSITY-WAVE;
TRANSITION; ANISOTROPY; BAFE2AS2; ORDER
AB We report the experimental details of how mechanical detwinning can be implemented in tandem with high-sensitivity nuclear magnetic resonance measurements and use this setup to measure the in-plane anisotropy of the spin-lattice relaxation rate in underdoped Ba(Fe1-x Co-x) As-2(2) with x = 0.048. The anisotropy reaches a maximum of 30% at T-N, and the recovery data reveal that the glassy behavior of the spin fluctuations present in the twinned state persist in the fully detwinned crystal. A theoretical model is presented to describe the spin-lattice relaxation rate in terms of anisotropic nematic spin fluctuations.
C1 [Kissikov, T.; Curro, N. J.] Univ Calif Davis, Dept Phys, Davis, CA 95616 USA.
[Dioguardi, A. P.] Los Alamos Natl Lab, Condensed Matter & Magnet Sci, POB 1663, Los Alamos, NM 87545 USA.
[Timmons, E. I.; Tanatar, M. A.; Prozorov, R.; Bud'ko, S. L.; Canfield, P. C.] Iowa State Univ, Ames Lab, US DOE, Ames, IA 50011 USA.
[Timmons, E. I.; Tanatar, M. A.; Prozorov, R.; Bud'ko, S. L.; Canfield, P. C.] Iowa State Univ, Dept Phys & Astron, Ames, IA 50011 USA.
[Fernandes, R. M.] Univ Minnesota, Sch Phys & Astron, Minneapolis, MN 55116 USA.
RP Kissikov, T (reprint author), Univ Calif Davis, Dept Phys, Davis, CA 95616 USA.
RI Fernandes, Rafael/E-9273-2010
FU NSF [DMR-1506961]; US Department of Energy, Office of Science, Basic
Energy Sciences [DE-SC0012336]; US Department of Energy, Office of Basic
Energy Science, Division of Materials Sciences and Engineering; US
Department of Energy by Iowa State University [DE-AC02-07CH11358];
National Science Foundation [PHY-1066293]
FX We thank S. Kivelson, E. Carlson, P. Pagliuso, and R. Urbano for
enlightening discussions and P. Klavins, J. Crocker, K. Shirer, and M.
Lawson for assistance in the laboratory. Work at UC Davis was supported
by the NSF under Grant No. DMR-1506961. R.M.F. is supported by the US
Department of Energy, Office of Science, Basic Energy Sciences, under
Award No. DE-SC0012336. Work done at Ames Laboratory (S.L.B., P.C.C.,
M.T., R.P., E.I.T.) was supported by the US Department of Energy, Office
of Basic Energy Science, Division of Materials Sciences and Engineering.
Ames Laboratory is operated for the US Department of Energy by Iowa
State University under Contract No. DE-AC02-07CH11358. This work was
completed at the Aspen Center for Physics, which is supported by the
National Science Foundation Grant No. PHY-1066293.
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SN 2469-9950
EI 2469-9969
J9 PHYS REV B
JI Phys. Rev. B
PD OCT 11
PY 2016
VL 94
IS 16
AR 165123
DI 10.1103/PhysRevB.94.165123
PG 8
WC Physics, Condensed Matter
SC Physics
GA DZ1UT
UT WOS:000385627200005
ER
PT J
AU Arnold, R
Augier, C
Baker, JD
Barabash, AS
Basharina-Freshville, A
Blondel, S
Blot, S
Bongrand, M
Brudanin, V
Busto, J
Caffrey, AJ
Calvez, S
Cascella, M
Cerna, C
Cesar, JP
Chapon, A
Chauveau, E
Chopra, A
Duchesneau, D
Durand, D
Egorov, V
Eurin, G
Evans, JJ
Fajt, L
Filosofov, D
Flack, R
Garrido, X
Gomez, H
Guillon, B
Guzowski, P
Hodak, R
Huber, A
Hubert, P
Hugon, C
Jullian, S
Klimenko, A
Kochetov, O
Konovalov, SI
Kovalenko, V
Lalanne, D
Lang, K
Lemiere, Y
Le Noblet, T
Liptak, Z
Liu, XR
Loaiza, P
Lutter, G
Mamedov, F
Marquet, C
Mauger, F
Morgan, B
Mott, J
Nemchenok, I
Nomachi, M
Nova, F
Nowacki, F
Ohsumi, H
Pahlka, RB
Perrot, F
Piquemal, F
Povinec, P
Pridal, P
Ramachers, YA
Remoto, A
Reyss, JL
Richards, B
Riddle, CL
Rukhadze, E
Saakyan, R
Salazar, R
Sarazin, X
Shitov, Y
Simard, L
Simkovic, F
Smetana, A
Smolek, K
Smolnikov, A
Soldner-Rembold, S
Soule, B
Stekl, I
Suhonen, J
Sutton, CS
Szklarz, G
Thomas, J
Timkin, V
Torre, S
Tretyak, VI
Tretyak, VI
Umatov, VI
Vanushin, I
Vilela, C
Vorobel, V
Waters, D
Zukauskas, A
AF Arnold, R.
Augier, C.
Baker, J. D.
Barabash, A. S.
Basharina-Freshville, A.
Blondel, S.
Blot, S.
Bongrand, M.
Brudanin, V.
Busto, J.
Caffrey, A. J.
Calvez, S.
Cascella, M.
Cerna, C.
Cesar, J. P.
Chapon, A.
Chauveau, E.
Chopra, A.
Duchesneau, D.
Durand, D.
Egorov, V.
Eurin, G.
Evans, J. J.
Fajt, L.
Filosofov, D.
Flack, R.
Garrido, X.
Gomez, H.
Guillon, B.
Guzowski, P.
Hodak, R.
Huber, A.
Hubert, P.
Hugon, C.
Jullian, S.
Klimenko, A.
Kochetov, O.
Konovalov, S. I.
Kovalenko, V.
Lalanne, D.
Lang, K.
Lemiere, Y.
Le Noblet, T.
Liptak, Z.
Liu, X. R.
Loaiza, P.
Lutter, G.
Mamedov, F.
Marquet, C.
Mauger, F.
Morgan, B.
Mott, J.
Nemchenok, I.
Nomachi, M.
Nova, F.
Nowacki, F.
Ohsumi, H.
Pahlka, R. B.
Perrot, F.
Piquemal, F.
Povinec, P.
Pridal, P.
Ramachers, Y. A.
Remoto, A.
Reyss, J. L.
Richards, B.
Riddle, C. L.
Rukhadze, E.
Saakyan, R.
Salazar, R.
Sarazin, X.
Shitov, Yu.
Simard, L.
Simkovic, F.
Smetana, A.
Smolek, K.
Smolnikov, A.
Soldner-Rembold, S.
Soule, B.
Stekl, I.
Suhonen, J.
Sutton, C. S.
Szklarz, G.
Thomas, J.
Timkin, V.
Torre, S.
Tretyak, Vl. I.
Tretyak, V. I.
Umatov, V. I.
Vanushin, I.
Vilela, C.
Vorobel, V.
Waters, D.
Zukauskas, A.
CA NEMO-3 Collaboration
TI Measurement of the 2 nu beta beta decay half-life of Nd-150 and a search
for 0 nu beta beta decay processes with the full exposure from the
NEMO-3 detector
SO PHYSICAL REVIEW D
LA English
DT Article
ID DOUBLE-BETA DECAY; TIME PROJECTION CHAMBER; NUCLEAR-DATA SHEETS;
2-BETA-2-NU DECAY; MAJORON
AB We present results from a search for neutrinoless double-beta (0 nu beta beta) decay using 36.6 g of the isotope Nd-150 with data corresponding to a live time of 5.25 y recorded with the NEMO-3 detector. We construct a complete background model for this isotope, including a measurement of the two-neutrino double-beta decay half-life of T-1/2(2 nu) = [9.34 +/- 0.22(stat)(-0.60)(+0.62)(syst)] x 10(18) y for the ground state transition, which represents the most precise result to date for this isotope. We perform a multivariate analysis to search for 0 nu beta beta decays in order to improve the sensitivity and, in the case of observation, disentangle the possible underlying decay mechanisms. As no evidence for 0 nu beta beta decay is observed, we derive lower limits on half-lives for several mechanisms involving physics beyond the standard model. The observed lower limit, assuming light Majorana neutrino exchange mediates the decay, is T-1/2(0 nu) > 2 > 2.0 x 10(22) y at the 90% C.L., corresponding to an upper limit on the effective neutrino mass of < m(nu)> < 1.6-5.3 eV.
C1 [Arnold, R.; Nowacki, F.] ULP, CNRS, IN2P3, IPHC, F-67037 Strasbourg, France.
[Augier, C.; Blondel, S.; Bongrand, M.; Calvez, S.; Eurin, G.; Garrido, X.; Gomez, H.; Jullian, S.; Lalanne, D.; Loaiza, P.; Sarazin, X.; Simard, L.; Szklarz, G.] Univ Paris Saclay, CNRS, IN2P3, Univ Paris 11,LAL, F-91405 Orsay, France.
[Baker, J. D.; Caffrey, A. J.; Riddle, C. L.] Idaho Natl Lab, Idaho Falls, ID 83415 USA.
[Barabash, A. S.; Konovalov, S. I.; Umatov, V. I.; Vanushin, I.] NRC Kurchatov Inst, ITEP, Moscow 117218, Russia.
[Basharina-Freshville, A.; Cascella, M.; Chopra, A.; Eurin, G.; Flack, R.; Liu, X. R.; Mott, J.; Richards, B.; Saakyan, R.; Thomas, J.; Torre, S.; Vilela, C.; Waters, D.] UCL, London WC1E 6BT, England.
[Blot, S.; Chauveau, E.; Evans, J. J.; Guzowski, P.; Soldner-Rembold, S.] Univ Manchester, Manchester M13 9PL, Lancs, England.
[Brudanin, V.; Egorov, V.; Filosofov, D.; Klimenko, A.; Kochetov, O.; Kovalenko, V.; Nemchenok, I.; Shitov, Yu.; Smolnikov, A.; Timkin, V.; Tretyak, V. I.] JINR, Dubna 141980, Russia.
[Brudanin, V.] Natl Res Nucl Univ, MEPhI, Moscow 115409, Russia.
[Busto, J.] Univ Marseille, CNRS, IN2P3, CPPM, F-13288 Marseille, France.
[Cerna, C.; Huber, A.; Hubert, P.; Hugon, C.; Lutter, G.; Marquet, C.; Perrot, F.; Piquemal, F.; Soule, B.] Univ Bordeaux, CNRS, IN2P3, CENBG, F-33175 Gradignan, France.
[Cesar, J. P.; Liptak, Z.; Nova, F.; Pahlka, R. B.; Salazar, R.] Univ Texas Austin, Austin, TX 78712 USA.
[Chapon, A.; Durand, D.; Guillon, B.; Lemiere, Y.; Mauger, F.] Univ Caen, CNRS, IN2P3, LPC Caen,ENSICAEN, F-14050 Caen, France.
[Duchesneau, D.; Le Noblet, T.; Remoto, A.] Univ Savoie, CNRS, IN2P3, LAPP, F-74941 Annecy Le Vieux, France.
[Fajt, L.; Hodak, R.; Mamedov, F.; Pridal, P.; Rukhadze, E.; Smetana, A.; Smolek, K.; Stekl, I.] Czech Tech Univ, Inst Expt & Appl Phys, CZ-12800 Prague, Czech Republic.
[Ramachers, Y. A.] Univ Warwick, Coventry CV4 7AL, W Midlands, England.
[Nomachi, M.] Osaka Univ, 1-1 Machikaney Arna Toyonaka, Osaka 5600043, Japan.
[Ohsumi, H.] Saga Univ, Saga 8408502, Japan.
[Piquemal, F.] Lab Souterrain Modane, F-73500 Modane, France.
[Povinec, P.; Simkovic, F.] Comenius Univ, FMFI, SK-84248 Bratislava, Slovakia.
[Reyss, J. L.] CNRS, LSCE, F-91190 Gif Sur Yvette, France.
[Shitov, Yu.] Univ London Imperial Coll Sci Technol & Med, London SW7 2AZ, England.
[Simard, L.] Inst Univ France, F-75005 Paris, France.
[Suhonen, J.] Univ Jyvaskyla, FIN-40351 Jyvaskyla, Finland.
[Sutton, C. S.] MHC, S Hadley, MA 01075 USA.
[Tretyak, Vl. I.] MSP, Inst Nucl Res, UA-03680 Kiev, Ukraine.
[Vorobel, V.; Zukauskas, A.] Charles Univ Prague, Fac Math & Phys, CZ-12116 Prague, Czech Republic.
RP Arnold, R (reprint author), ULP, CNRS, IN2P3, IPHC, F-67037 Strasbourg, France.
RI Barabash, Alexander/S-8851-2016;
OI Remoto, Alberto/0000-0001-9413-0356
FU Czech Republic; National Center for Scientific Research/National
Institute of Nuclear and Particle Physics (France); Russian Foundation
for Basic Research (Russia); Science and Technology Facilities Council
(United Kingdom); National Science Foundation (United States)
FX The authors thank the staffs of the Modane Underground Laboratory for
their technical assistance in operating the detector. We acknowledge
support by the funding agencies of the Czech Republic, the National
Center for Scientific Research/National Institute of Nuclear and
Particle Physics (France), the Russian Foundation for Basic Research
(Russia), the Science and Technology Facilities Council (United
Kingdom), and the National Science Foundation (United States).
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PI COLLEGE PK
PA ONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA
SN 2470-0010
EI 2470-0029
J9 PHYS REV D
JI Phys. Rev. D
PD OCT 11
PY 2016
VL 94
IS 7
AR 072003
DI 10.1103/PhysRevD.94.072003
PG 19
WC Astronomy & Astrophysics; Physics, Particles & Fields
SC Astronomy & Astrophysics; Physics
GA DZ1WJ
UT WOS:000385632000002
ER
PT J
AU Chen, XM
Thampy, V
Mazzoli, C
Barbour, AM
Miao, H
Gu, GD
Cao, Y
Tranquada, JM
Dean, MPM
Wilkins, SB
AF Chen, X. M.
Thampy, V.
Mazzoli, C.
Barbour, A. M.
Miao, H.
Gu, G. D.
Cao, Y.
Tranquada, J. M.
Dean, M. P. M.
Wilkins, S. B.
TI Remarkable Stability of Charge Density Wave Order in La1.875Ba0.125CuO4
SO PHYSICAL REVIEW LETTERS
LA English
DT Article
ID INTENSITY FLUCTUATION SPECTROSCOPY; T-C SUPERCONDUCTOR;
X-RAY-SCATTERING; CUPRATE SUPERCONDUCTORS; FERMI-SURFACE; NORMAL-STATE;
LA2-XBAXCUO4; YBA2CU3O6.67; INSTABILITY; COLLOQUIUM
AB The occurrence of charge-density-wave (CDW) order in underdoped cuprates is now well established, although the precise nature of the CDW and its relationship with superconductivity is not. Theoretical proposals include contrasting ideas such as that pairing may be driven by CDW fluctuations or that static CDWs may intertwine with a spatially modulated superconducting wave function. We test the dynamics of CDW order in La1.825Ba0.125CuO4 by using x-ray photon correlation spectroscopy at the CDW wave vector, detected resonantly at the Cu L-3 edge. We find that the CDW domains are strikingly static, with no evidence of significant fluctuations up to 2 (3)/(4) h. We discuss the implications of these results for some of the competing theories.
C1 [Chen, X. M.; Thampy, V.; Miao, H.; Gu, G. D.; Cao, Y.; Tranquada, J. M.; Dean, M. P. M.] Brookhaven Natl Lab, Condensed Matter Phys & Mat Sci Dept, Upton, NY 11973 USA.
[Mazzoli, C.; Barbour, A. M.; Wilkins, S. B.] Brookhaven Natl Lab, Natl Synchrotron Light Source 2, Upton, NY 11973 USA.
RP Chen, XM (reprint author), Brookhaven Natl Lab, Condensed Matter Phys & Mat Sci Dept, Upton, NY 11973 USA.
EM xmchen@bnl.gov; vthampy@bnl.gov; mdean@bnl.gov; swilkins@bnl.gov
RI Dean, Mark/B-4541-2011; Tranquada, John/A-9832-2009
OI Dean, Mark/0000-0001-5139-3543; Tranquada, John/0000-0003-4984-8857
FU US Department of Energy, Division of Materials Science [DE-SC00112704];
Center for Emergent Superconductivity, an Energy Frontier Research
Center - U.S. DOE, Office of Basic Energy Sciences; DOE Office of
Science [DE-SC0012704]
FX We thank Mark Sutton for his insightful comments regarding speckle
visibility and Gilberto Fabbris and John Hill for discussion about
stripe correlations in the cuprates. Work performed at Brookhaven
National Laboratory was supported by the US Department of Energy,
Division of Materials Science, under Contract No. DE-SC00112704. X-ray
scattering measurements by H. M., M. P. M. D., and J. M. T. were
supported by the Center for Emergent Superconductivity, an Energy
Frontier Research Center funded by the U.S. DOE, Office of Basic Energy
Sciences. This research used resources at the 23-ID-1 beam line of the
National Synchrotron Light Source II, a U.S. Department of Energy (DOE)
Office of Science User Facility operated for the DOE Office of Science
by Brookhaven National Laboratory under Contract No. DE-SC0012704. X. M.
Chen and V. Thampy contributed equally to this work.
NR 69
TC 1
Z9 1
U1 18
U2 18
PU AMER PHYSICAL SOC
PI COLLEGE PK
PA ONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA
SN 0031-9007
EI 1079-7114
J9 PHYS REV LETT
JI Phys. Rev. Lett.
PD OCT 11
PY 2016
VL 117
IS 16
AR 167001
DI 10.1103/PhysRevLett.117.167001
PG 6
WC Physics, Multidisciplinary
SC Physics
GA DZ1ZP
UT WOS:000385641300014
PM 27792368
ER
PT J
AU Lo Vecchio, I
Denlinger, JD
Krupin, O
Kim, BJ
Metcalf, PA
Lupi, S
Allen, JW
Lanzara, A
AF Lo Vecchio, I.
Denlinger, J. D.
Krupin, O.
Kim, B. J.
Metcalf, P. A.
Lupi, S.
Allen, J. W.
Lanzara, A.
TI Fermi Surface of Metallic V2O3 from Angle-Resolved Photoemission:
Mid-level Filling of e(g)(pi) Bands
SO PHYSICAL REVIEW LETTERS
LA English
DT Article
ID MEAN-FIELD THEORY; INSULATOR-TRANSITION; DOPED V2O3; PHASE
AB Using angle resolved photoemission spectroscopy, we report the first band dispersions and distinct features of the bulk Fermi surface (FS) in the paramagnetic metallic phase of the prototypical metal-insulator transition material V2O3. Along the c axis we observe both an electron pocket and a triangular holelike FS topology, showing that both V 3d a(1g) and e(g)(pi) states contribute to the FS. These results challenge the existing correlation-enhanced crystal field splitting theoretical explanation for the transition mechanism and pave the way for the solution of this mystery.
C1 [Lo Vecchio, I.; Lanzara, A.] Lawrence Berkeley Natl Lab, Div Mat Sci, Berkeley, CA 94720 USA.
[Denlinger, J. D.; Krupin, O.] Lawrence Berkeley Natl Lab, Adv Light Source, Berkeley, CA 94720 USA.
[Kim, B. J.] Max Planck Inst Festkorperforsch, Heisenbergstr 1, D-70569 Stuttgart, Germany.
[Metcalf, P. A.] Purdue Univ, Sch Mat Engn, W Lafayette, IN 47907 USA.
[Lupi, S.] Univ Roma Sapienza, CNR IOM, I-00185 Rome, Italy.
[Lupi, S.] Univ Roma Sapienza, Dipartimento Fis, I-00185 Rome, Italy.
[Allen, J. W.] Univ Michigan, Randall Lab Phys, Ann Arbor, MI 48109 USA.
[Lanzara, A.] Univ Calif Berkeley, Dept Phys, Berkeley, CA 94720 USA.
RP Denlinger, JD (reprint author), Lawrence Berkeley Natl Lab, Adv Light Source, Berkeley, CA 94720 USA.
EM jddenlinger@lbl.gov; alanzara@lbl.gov
FU Advanced Light Source (ALS); National Science Foundation [DMR-1410660];
Office of Science of the U.S. Department of Energy [DE-AC02-05CH11231]
FX We gratefully acknowledge theoretical advice and stimulating discussions
with Byung Il Min, Richard Martin, and especially Frank Lechermann. J.
W. A. thanks the Advanced Light Source (ALS) for supporting a visit to
the ALS during the time that this paper was written. This work was
supported by the National Science Foundation Grant No. DMR-1410660.
Theory calculations used resources of the National Energy Research
Scientific Computing Center (NERSC). Both the ALS and NERSC user
facilities are supported by the Office of Science of the U.S. Department
of Energy under Contract No. DE-AC02-05CH11231.
NR 32
TC 0
Z9 0
U1 12
U2 12
PU AMER PHYSICAL SOC
PI COLLEGE PK
PA ONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA
SN 0031-9007
EI 1079-7114
J9 PHYS REV LETT
JI Phys. Rev. Lett.
PD OCT 11
PY 2016
VL 117
IS 16
AR 166401
DI 10.1103/PhysRevLett.117.166401
PG 5
WC Physics, Multidisciplinary
SC Physics
GA DZ1ZP
UT WOS:000385641300009
PM 27792364
ER
PT J
AU Boden, R
Hutt, LP
Huntemann, M
Clum, A
Pillay, M
Palaniappan, K
Varghese, N
Mikhailova, N
Stamatis, D
Reddy, T
Ngan, CY
Daum, C
Shapiro, N
Markowitz, V
Ivanova, N
Woyke, T
Kyrpides, N
AF Boden, Rich
Hutt, Lee P.
Huntemann, Marcel
Clum, Alicia
Pillay, Manoj
Palaniappan, Krishnaveni
Varghese, Neha
Mikhailova, Natalia
Stamatis, Dimitrios
Reddy, Tatiparthi
Ngan, Chew Yee
Daum, Chris
Shapiro, Nicole
Markowitz, Victor
Ivanova, Natalia
Woyke, Tanja
Kyrpides, Nikos
TI Permanent draft genome of Thermithiobacillus tepidarius DSM 3134(T), a
moderately thermophilic, obligately chemolithoautotrophic member of the
Acidithiobacillia (vol 11, 74, 2016)
SO STANDARDS IN GENOMIC SCIENCES
LA English
DT Correction
C1 [Boden, Rich; Hutt, Lee P.] Univ Plymouth, Sch Biol Sci, Drake Circus, Plymouth PL4 8AA, Devon, England.
[Boden, Rich; Hutt, Lee P.] Univ Plymouth, Sustainable Earth Inst, Drake Circus, Plymouth PL4 8AA, Devon, England.
[Huntemann, Marcel; Clum, Alicia; Pillay, Manoj; Palaniappan, Krishnaveni; Varghese, Neha; Mikhailova, Natalia; Stamatis, Dimitrios; Reddy, Tatiparthi; Ngan, Chew Yee; Daum, Chris; Shapiro, Nicole; Markowitz, Victor; Ivanova, Natalia; Woyke, Tanja; Kyrpides, Nikos] DOE Joint Genome Inst, Walnut Creek, CA 94598 USA.
RP Boden, R (reprint author), Univ Plymouth, Sch Biol Sci, Drake Circus, Plymouth PL4 8AA, Devon, England.; Boden, R (reprint author), Univ Plymouth, Sustainable Earth Inst, Drake Circus, Plymouth PL4 8AA, Devon, England.
EM rich.boden@plymouth.ac.uk
RI Kyrpides, Nikos/A-6305-2014
OI Kyrpides, Nikos/0000-0002-6131-0462
NR 1
TC 0
Z9 0
U1 2
U2 2
PU BIOMED CENTRAL LTD
PI LONDON
PA 236 GRAYS INN RD, FLOOR 6, LONDON WC1X 8HL, ENGLAND
SN 1944-3277
J9 STAND GENOMIC SCI
JI Stand. Genomic Sci.
PD OCT 11
PY 2016
VL 11
AR 77
DI 10.1186/s40793-016-0197-z
PG 1
WC Genetics & Heredity; Microbiology
SC Genetics & Heredity; Microbiology
GA DY7OC
UT WOS:000385317600001
PM 27777647
ER
PT J
AU Gupta, S
Fischer, JKH
Lunkenheimer, P
Loidl, A
Novak, E
Jalarvo, N
Ohl, M
AF Gupta, S.
Fischer, J. K. H.
Lunkenheimer, P.
Loidl, A.
Novak, E.
Jalarvo, N.
Ohl, M.
TI Effect of adding nanometre-sized heterogeneities on the structural
dynamics and the excess wing of a molecular glass former
SO SCIENTIFIC REPORTS
LA English
DT Article
ID NEUTRON SPIN-ECHO; GOLDSTEIN BETA-RELAXATION; SUPERCOOLED LIQUIDS;
DIELECTRIC-SPECTROSCOPY; SECONDARY RELAXATIONS; FORMING LIQUIDS; LENGTH
SCALE; TRANSITION; ALPHA; GLYCEROL
AB We present the relaxation dynamics of glass-forming glycerol mixed with 1.1 nm sized polyhedral oligomeric silsesquioxane (POSS) molecules using dielectric spectroscopy (DS) and two different neutron scattering (NS) techniques. Both, the reorientational dynamics as measured by DS and the density fluctuations detected by NS reveal a broadening of the alpha relaxation when POSS molecules are added. Moreover, we find a significant slowing down of the alpha-relaxation time. These effects are in accord with the heterogeneity scenario considered for the dynamics of glasses and supercooled liquids. The addition of POSS also affects the excess wing in glycerol arising from a secondary relaxation process, which seems to exhibit a dramatic increase in relative strength compared to the alpha relaxation.
C1 [Gupta, S.; Jalarvo, N.; Ohl, M.] Juelich Ctr Neutron Sci JCNS Outstn SNS, POB 2008,1 Bethel Valley Rd, Oak Ridge, TN 37831 USA.
[Gupta, S.; Ohl, M.] Oak Ridge Natl Lab, Neutron Sci Directorate, Biol & Soft Matter Div, POB 2008,1 Bethel Valley Rd, Oak Ridge, TN 37831 USA.
[Gupta, S.] Louisiana State Univ, Dept Chem, Baton Rouge, LA 70803 USA.
[Gupta, S.] Louisiana State Univ, Macromol Studies Grp, Baton Rouge, LA 70803 USA.
[Fischer, J. K. H.; Lunkenheimer, P.; Loidl, A.] Univ Augsburg, Ctr Elect Correlat & Magnetism, Expt Phys 5, D-86135 Augsburg, Germany.
[Novak, E.] Univ Tennessee, Dept Mat Sci & Engn, Knoxville, TN 37996 USA.
[Jalarvo, N.] Oak Ridge Natl Lab, Chem & Engn Mat Div, POB 2008 MS6473, Oak Ridge, TN 37831 USA.
RP Gupta, S (reprint author), Juelich Ctr Neutron Sci JCNS Outstn SNS, POB 2008,1 Bethel Valley Rd, Oak Ridge, TN 37831 USA.; Gupta, S (reprint author), Oak Ridge Natl Lab, Neutron Sci Directorate, Biol & Soft Matter Div, POB 2008,1 Bethel Valley Rd, Oak Ridge, TN 37831 USA.; Gupta, S (reprint author), Louisiana State Univ, Dept Chem, Baton Rouge, LA 70803 USA.; Gupta, S (reprint author), Louisiana State Univ, Macromol Studies Grp, Baton Rouge, LA 70803 USA.
EM sudiptag@lsu.edu
RI Lunkenheimer, Peter/C-6196-2008; Fischer, Jonas K. H./P-2505-2014;
Loidl, Alois/L-8199-2015;
OI Lunkenheimer, Peter/0000-0002-4525-1394; Fischer, Jonas K.
H./0000-0001-8129-0713; Loidl, Alois/0000-0002-5579-0746; Jalarvo,
Niina/0000-0003-0644-6866
FU Scientific User Facilities Division, Office of Basic Energy Sciences, US
Department of Energy (DOE)
FX SG thanks R. Zorn for helpful discussions. We thank S. V. Pingali for
helping us with the SANS experiment. Research conducted at ORNL's
Spallation Neutron Source (SNS) and High Flux Isotope Reactor (HFIR) was
sponsored by the Scientific User Facilities Division, Office of Basic
Energy Sciences, US Department of Energy (DOE).
NR 63
TC 1
Z9 1
U1 10
U2 10
PU NATURE PUBLISHING GROUP
PI LONDON
PA MACMILLAN BUILDING, 4 CRINAN ST, LONDON N1 9XW, ENGLAND
SN 2045-2322
J9 SCI REP-UK
JI Sci Rep
PD OCT 11
PY 2016
VL 6
AR 35034
DI 10.1038/srep35034
PG 12
WC Multidisciplinary Sciences
SC Science & Technology - Other Topics
GA DY4IX
UT WOS:000385063300001
PM 27725747
ER
PT J
AU Purevjav, N
Okuchi, T
Tomioka, N
Wang, XP
Hoffmann, C
AF Purevjav, Narangoo
Okuchi, Takuo
Tomioka, Naotaka
Wang, Xiaoping
Hoffmann, Christina
TI Quantitative analysis of hydrogen sites and occupancy in deep mantle
hydrous wadsleyite using single crystal neutron diffraction
SO SCIENTIFIC REPORTS
LA English
DT Article
ID FE-BEARING WADSLEYITE; EARTHS UPPER-MANTLE; X-RAY-DIFFRACTION;
TRANSITION-ZONE; SYSTEM MG2SIO4-FE2SIO4; SEISMIC DISCONTINUITY; ELASTIC
PROPERTIES; SOUND VELOCITIES; MODIFIED SPINEL; GAMMA-PHASE
AB Evidence from seismological and mineralogical studies increasingly indicates that water from the oceans has been transported to the deep earth to form water-bearing dense mantle minerals. Wadsleyite [(Mg, Fe2+)(2)SiO4] has been identified as one of the most important host minerals incorporating this type of water, which is capable of storing the entire mass of the oceans as a hidden reservoir. To understand the effects of such water on the physical properties and chemical evolution of Earth's interior, it is essential to determine where in the crystal structure the hydration occurs and which chemical bonds are altered and weakened after hydration. Here, we conduct a neutron time-of-flight single-crystal Laue diffraction study on hydrous wadsleyite. Single crystals were grown under pressure to a size suitable for the experiment and with physical qualities representative of wet, deep mantle conditions. The results of this neutron single crystal diffraction study unambiguously demonstrate the method of hydrogen incorporation into the wadsleyite, which is qualitatively different from that of its denser polymorph, ringwoodite, in the wet mantle. The difference is a vital clue towards understanding why these dense mantle minerals show distinctly different softening behaviours after hydration.
C1 [Purevjav, Narangoo; Okuchi, Takuo; Tomioka, Naotaka] Okayama Univ, Inst Planetary Mat, Misasa, Tottori 6820193, Japan.
[Tomioka, Naotaka] Japan Agcy Marine Earth Sci & Technol, Kochi Inst Core Sample Res, Nankoku, Kochi 7838502, Japan.
[Wang, Xiaoping; Hoffmann, Christina] Oak Ridge Natl Lab, Neutron Sci Directorate, Chem & Engn Mat Div, Oak Ridge, TN 37831 USA.
RP Purevjav, N (reprint author), Okayama Univ, Inst Planetary Mat, Misasa, Tottori 6820193, Japan.
EM pxec5a1c@s.okayama-u.ac.jp
RI OKUCHI, Takuo/B-1884-2011; Tomioka, Naotaka/B-1888-2011
OI OKUCHI, Takuo/0000-0001-6907-0945; Tomioka, Naotaka/0000-0001-5725-9513
FU Scientific User Facilities Division, Office of Basic Energy Sciences, U.
S. Department of Energy; JSPS KAKENHI [26287135, 15J03633, 15K13593]
FX We thank C. Oka and S. Yamashita for technical support during
high-pressure synthesis and FTIR measurement, respectively. Part of the
research conducted at Oak Ridge National Laboratory's Spallation Neutron
Source was sponsored by the Scientific User Facilities Division, Office
of Basic Energy Sciences, U. S. Department of Energy. This work was
supported by JSPS KAKENHI Grant Numbers 26287135, 15J03633 and 15K13593.
NR 51
TC 0
Z9 0
U1 9
U2 9
PU NATURE PUBLISHING GROUP
PI LONDON
PA MACMILLAN BUILDING, 4 CRINAN ST, LONDON N1 9XW, ENGLAND
SN 2045-2322
J9 SCI REP-UK
JI Sci Rep
PD OCT 11
PY 2016
VL 6
AR 34988
DI 10.1038/srep34988
PG 8
WC Multidisciplinary Sciences
SC Science & Technology - Other Topics
GA DY6MG
UT WOS:000385240800002
PM 27725749
ER
PT J
AU Pujol, A
Chang, C
Naga, EG
Amara, A
Refregier, A
Bacon, DJ
Carretero, J
Castander, FJ
Crocce, M
Fosalba, P
Manera, M
Vikram, V
AF Pujol, Arnau
Chang, Chihway
Naga, Enrique Gazta
Amara, Adam
Refregier, Alexandre
Bacon, David J.
Carretero, Jorge
Castander, Francisco J.
Crocce, Martin
Fosalba, Pablo
Manera, Marc
Vikram, Vinu
TI A new method to measure galaxy bias by combining the density and weak
lensing fields
SO MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
LA English
DT Article
DE gravitational lensing: weak; surveys; large-scale structure of Universe
ID LARGE-SCALE BIAS; CHALLENGE LIGHTCONE SIMULATION; PEAK-BACKGROUND SPLIT;
DARK-MATTER HALOES; PERTURBATION-THEORY; ASSEMBLY BIAS; PARAMETER
CONSTRAINTS; LUMINOSITY FUNCTION; DEEP SURVEY; MODEL
AB We present a newmethod to measure redshift-dependent galaxy bias by combining information from the galaxy density field and the weak lensing field. This method is based on the work of Amara et al., who use the galaxy density field to construct a bias-weighted convergence field kappa(g). The main difference between Amara et al.'s work and our new implementation is that here we present another way to measure galaxy bias, using tomography instead of bias parametrizations. The correlation between kappa(g) and the true lensing field. allows us to measure galaxy bias using different zero-lag correlations, such as / or / . Our method measures the linear bias factor on linear scales, under the assumption of no stochasticity between galaxies and matter. We use the Marenostrum Institut de Ciencies de l'Espai (MICE) simulation tomeasure the linear galaxy bias for a flux-limited sample (i<22.5) in tomographic redshift bins using this method. This article is the first that studies the accuracy and systematic uncertainties associated with the implementation of the method and the regime in which it is consistent with the linear galaxy bias defined by projected two-point correlation functions (2PCF). We find that our method is consistent with a linear bias at the per cent level for scales larger than 30 arcmin, while non-linearities appear at smaller scales. This measurement is a good complement to other measurements of bias, since it does not depend strongly on sigma(8) as do the 2PCF measurements. We will apply this method to the Dark Energy Survey Science Verification data in a follow-up article.
C1 [Pujol, Arnau; Naga, Enrique Gazta; Carretero, Jorge; Castander, Francisco J.; Crocce, Martin; Fosalba, Pablo] IEEC CSIC, ICE, E-08193 Barcelona, Spain.
[Chang, Chihway; Amara, Adam; Refregier, Alexandre] Swiss Fed Inst Technol, Dept Phys, Wolfgang Pauli Str 16, CH-8093 Zurich, Switzerland.
[Bacon, David J.] Univ Portsmouth, Inst Cosmol & Gravitat, Dennis Sciama Bldg, Portsmouth PO1 3FX, Hants, England.
[Carretero, Jorge] Univ Autonoma Barcelona, Inst Fis Altes Energies, E-08193 Barcelona, Spain.
[Manera, Marc] UCL, Gower St, London WC1E 6BT, England.
[Vikram, Vinu] Argonne Natl Lab, 9700 South Cass Ave, Argonne, IL 60439 USA.
[Vikram, Vinu] Univ Penn, Dept Astron & Astrophys, Philadelphia, PA 19104 USA.
RP Pujol, A (reprint author), IEEC CSIC, ICE, E-08193 Barcelona, Spain.
EM arnaupv@gmail.com
RI Gaztanaga, Enrique/L-4894-2014
OI Gaztanaga, Enrique/0000-0001-9632-0815
FU Spanish Ministerio de Ciencia e Innovacion (MICINN) [200850I176,
AYA2009-13936, AYA2012-39620, AYA2013-44327, ESP2013-48274,
ESP2014-58384]; Consolider-Ingenio [CSD2007-00060]; Generalitat de
Catalunya [2009-SGR-1398]; Ramon y Cajal MICINN program; beca FI; MICINN
[AYA2012-39620]; Swiss National Science Foundation [200021-149442,
200021-143906]; MINECO [ESP2013-48274-C3-1-P]; [AECT-2006-2-0011];
[AECT-2006-2-0012]; [AECT-2015-1-0013]
FX We thank Juan Garcia-Bellido for the final revision of the article. The
MICE simulations have been developed at the MareNostrum supercomputer
(BSC-CNS) thanks to grants AECT-2006-2-0011 through AECT-2015-1-0013.
Data products have been stored at the Port d'Informacio Cientifica (PIC)
and distributed through the CosmoHub webportal (cosmohub.pic.es).
Funding for this project was partially provided by the Spanish
Ministerio de Ciencia e Innovacion (MICINN), projects 200850I176,
AYA2009-13936, AYA2012-39620, AYA2013-44327, ESP2013-48274,
ESP2014-58384, Consolider-Ingenio CSD2007-00060, research project
2009-SGR-1398 from Generalitat de Catalunya and the Ramon y Cajal MICINN
program. AP was supported by beca FI and 2009-SGR-1398 from Generalitat
de Catalunya and project AYA2012-39620 from MICINN. CC, AA and AR are
supported by the Swiss National Science Foundation grants 200021-149442
and 200021-143906. PF is funded by MINECO, project ESP2013-48274-C3-1-P.
NR 73
TC 3
Z9 3
U1 0
U2 0
PU OXFORD UNIV PRESS
PI OXFORD
PA GREAT CLARENDON ST, OXFORD OX2 6DP, ENGLAND
SN 0035-8711
EI 1365-2966
J9 MON NOT R ASTRON SOC
JI Mon. Not. Roy. Astron. Soc.
PD OCT 11
PY 2016
VL 462
IS 1
BP 35
EP 47
DI 10.1093/mnras/stw1612
PG 13
WC Astronomy & Astrophysics
SC Astronomy & Astrophysics
GA DW3BI
UT WOS:000383516700029
ER
PT J
AU Bhat, P
Ebrahimi, F
Blackman, EG
AF Bhat, Pallavi
Ebrahimi, Fatima
Blackman, Eric G.
TI Large-scale dynamo action precedes turbulence in shearing box
simulations of the magnetorotational instability
SO MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
LA English
DT Article
DE accretion, accretion discs; dynamo; magnetic fields; MHD; turbulence
ID STRATIFIED ACCRETION DISKS; WEAKLY MAGNETIZED DISKS; MEAN-FIELD DYNAMO;
LOCAL SIMULATIONS; SATURATION; CONVERGENCE; MODELS; LIMIT; FLUX; FLOW
AB We study the dynamo generation (exponential growth) of large-scale (planar averaged) fields in unstratified shearing box simulations of the magnetorotational instability (MRI). In contrast to previous studies restricted to horizontal (x-y) averaging, we also demonstrate the presence of large-scale fields when vertical (y-z) averaging is employed instead. By computing space-time planar averaged fields and power spectra, we find large-scale dynamo action in the early MRI growth phase - a previously unidentified feature. Non-axisymmetric linear MRI modes with low horizontal wavenumbers and vertical wavenumbers near that of expected maximal growth, amplify the large-scale fields exponentially before turbulence and high wavenumber fluctuations arise. Thus the large-scale dynamo requires only linear fluctuations but not non-linear turbulence (as defined by mode-mode coupling). Vertical averaging also allows for monitoring the evolution of the large-scale vertical field and we find that a feedback from horizontal low wavenumber MRI modes provides a clue as to why the large-scale vertical field sustains against turbulent diffusion in the non-linear saturation regime. We compute the terms in the mean field equations to identify the individual contributions to large-scale field growth for both types of averaging. The large-scale fields obtained from vertical averaging are found to compare well with global simulations and quasi-linear analytical analysis from a previous study by Ebrahimi & Blackman. We discuss the potential implications of these new results for understanding the large-scale MRI dynamo saturation and turbulence.
C1 [Bhat, Pallavi; Ebrahimi, Fatima] Princeton Univ, Dept Astrophys Sci, Princeton, NJ 08543 USA.
[Bhat, Pallavi; Ebrahimi, Fatima] Princeton Univ, Princeton Plasma Phys Lab, POB 451, Princeton, NJ 08543 USA.
[Blackman, Eric G.] Univ Rochester, Dept Phys & Astron, Rochester, NY 14618 USA.
RP Bhat, P (reprint author), Princeton Univ, Dept Astrophys Sci, Princeton, NJ 08543 USA.; Bhat, P (reprint author), Princeton Univ, Princeton Plasma Phys Lab, POB 451, Princeton, NJ 08543 USA.
EM pbhat@princeton.edu; ebrahimi@princeton.edu; black-man@pas.rochester.edu
FU DOE [DE-SC0012467]; [HST-AR-13916.002]; [NSF AST1515648]
FX We acknowledge useful insights from K. Subramanian and useful
discussions with F. Nauman. PB and FE acknowledge grant support from
DOE, DE-SC0012467. EB acknowledges support from grants HST-AR-13916.002,
and NSF AST1515648. The computing resources were provided by Princeton
Institute of Computational Science (PICSciE).
NR 38
TC 1
Z9 1
U1 1
U2 1
PU OXFORD UNIV PRESS
PI OXFORD
PA GREAT CLARENDON ST, OXFORD OX2 6DP, ENGLAND
SN 0035-8711
EI 1365-2966
J9 MON NOT R ASTRON SOC
JI Mon. Not. Roy. Astron. Soc.
PD OCT 11
PY 2016
VL 462
IS 1
BP 818
EP 829
DI 10.1093/mnras/stw1619
PG 12
WC Astronomy & Astrophysics
SC Astronomy & Astrophysics
GA DW3BI
UT WOS:000383516700088
ER
PT J
AU Gu, WQ
Cao, GF
Chen, XH
Ji, XP
Li, GS
Ling, JJ
Liu, J
Qian, X
Wang, W
AF Gu, W. Q.
Cao, G. F.
Chen, X. H.
Ji, X. P.
Li, G. S.
Ling, J. J.
Liu, J.
Qian, X.
Wang, W.
TI Background evaluation for the neutron sources in the Daya Bay experiment
SO NUCLEAR INSTRUMENTS & METHODS IN PHYSICS RESEARCH SECTION A-ACCELERATORS
SPECTROMETERS DETECTORS AND ASSOCIATED EQUIPMENT
LA English
DT Article
DE theta(13); Reactor neutrino; Inverse-beta decay; Am-241-C-13 neutron
source; Background
ID SYSTEM
AB We present an evaluation of the background induced by Am-241-C-13 neutron calibration sources in the Daya Bay reactor neutrino experiment. As a significant background for electron-antineutrino detection at 0.26 +/- 0.12 per detector per day on average, it has been estimated by a Monte Carlo simulation that was benchmarked by a special calibration data set. This dedicated data set also provides the energy spectrum of the background. (C) 2016 Elsevier B.V. All rights reserved.
C1 [Gu, W. Q.; Li, G. S.; Liu, J.] Shanghai Jiao Tong Univ, Dept Phys & Astron, Shanghai Lab Particle Phys & Cosmol, Shanghai, Peoples R China.
[Ji, X. P.] Tsinghua Univ, Dept Engn Phys, Beijing, Peoples R China.
[Cao, G. F.; Chen, X. H.] Inst High Energy Phys, Beijing, Peoples R China.
[Ling, J. J.; Qian, X.] Brookhaven Natl Lab, Upton, NY USA.
[Ling, J. J.; Wang, W.] Sun Yat Sen Zhongshan Univ, Guangzhou, Guangdong, Peoples R China.
[Ji, X. P.] Nankai Univ, Sch Phys, Tianjin, Peoples R China.
[Ling, J. J.] Univ Illinois, Dept Phys, Urbana, IL USA.
[Wang, W.] Coll William & Mary, Williamsburg, VA USA.
RP Gu, WQ (reprint author), Shanghai Jiao Tong Univ, Dept Phys & Astron, Shanghai Lab Particle Phys & Cosmol, Shanghai, Peoples R China.
EM wenqiang.gu@sjtu.edu.cn; jianglai.liu@sjtu.edu.cn
RI Ling, Jiajie/I-9173-2014; Liu, Jianglai/P-2587-2015
OI Ling, Jiajie/0000-0003-2982-0670; Liu, Jianglai/0000-0002-4563-3157
FU Natural Science Foundation of China [11175116]; Chinese Ministry of
Science and Technology grant [2013CB834306]; Shanghai Laboratory for
Particle Physics and Cosmology at the Shanghai Jiao Tong University; CAS
Center for Excellence in Particle Physics (CCEPP)
FX This work was done with support from the Natural Science Foundation of
China grants 11175116, the Chinese Ministry of Science and Technology
grant 2013CB834306, Shanghai Laboratory for Particle Physics and
Cosmology at the Shanghai Jiao Tong University, and the CAS Center for
Excellence in Particle Physics (CCEPP). We gratefully thank X.L. Chen
from China Institute of Atomic Energy for the preparation of the
high-activity 241Am-13C source.
NR 16
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PI AMSTERDAM
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SN 0168-9002
EI 1872-9576
J9 NUCL INSTRUM METH A
JI Nucl. Instrum. Methods Phys. Res. Sect. A-Accel. Spectrom. Dect. Assoc.
Equip.
PD OCT 11
PY 2016
VL 833
BP 27
EP 32
DI 10.1016/j.nima.2016.07.007
PG 6
WC Instruments & Instrumentation; Nuclear Science & Technology; Physics,
Nuclear; Physics, Particles & Fields
SC Instruments & Instrumentation; Nuclear Science & Technology; Physics
GA DW7GC
UT WOS:000383818200005
ER
PT J
AU Knowles, J
Skutnik, S
Glasgow, D
Kapsimalis, R
AF Knowles, Justin
Skutnik, Steven
Glasgow, David
Kapsimalis, Roger
TI A generalized method for characterization of U-235 and Pu-239 content
using short-lived fission product gamma spectroscopy
SO NUCLEAR INSTRUMENTS & METHODS IN PHYSICS RESEARCH SECTION A-ACCELERATORS
SPECTROMETERS DETECTORS AND ASSOCIATED EQUIPMENT
LA English
DT Article
DE Gamma spectroscopy; Short-lived fission products; Neutron Activation
Analysis; Nuclear forensics; Safeguards; ORIGEN
ID SCALE
AB Rapid nondestructive assay methods for trace fissile material analysis are needed in both nuclear forensics and safeguards communities. To address these needs, research at the Oak Ridge National Laboratory High Flux Isotope Reactor Neutron Activation Analysis facility has developed a generalized nondestructive assay method to characterize materials containing fissile isotopes. This method relies on gamma-ray emissions from short-lived fission products and makes use of differences in fission product yields to identify fissile compositions of trace material samples. Although prior work has explored the use of short-lived fission product gamma-ray measurements, the proposed method is the first to provide a complete characterization of isotopic identification, mass ratios, and absolute mass determination. Successful single fissile isotope mass recoveries of less than 6% recovery bias have been conducted on standards of U-235 and Pu-239 as low as 12 ng in less than 10 minutes. Additionally, mixtures of fissile isotope standards containing U-235 and Pu-239 have been characterized as low as 198 ng of fissile mass with less than 7% recovery bias. The generalizability of this method is illustrated by evaluating different fissile isotopes, mixtures Of fissile isotopes, and two different irradiation positions in the reactor. It is anticipated that this method will be expanded to characterize additional fissile nuclides, utilize various irradiation facilities, and account for increasingly complex sample matrices. (C) 2016 The Authors. Published by Elsevier B.V.
C1 [Knowles, Justin; Skutnik, Steven] Univ Tennessee, Knoxville, TN 37996 USA.
[Glasgow, David; Kapsimalis, Roger] Oak Ridge Natl Lab, Oak Ridge, TN USA.
RP Knowles, J (reprint author), Univ Tennessee, Knoxville, TN 37996 USA.
EM knowles@utk.edu
FU University of Tennessee/Oak Ridge National Laboratory Bredesen Center
for Interdisciplinary Research and Graduate Education; U.S. Department
of Energy [DE-AC05-00OR22725]
FX The authors would like to recognize fellowship support from the
University of Tennessee/Oak Ridge National Laboratory Bredesen Center
for Interdisciplinary Research and Graduate Education. In addition, this
research has been made possible by facilities at the Oak Ridge National
Laboratory, managed by UT-Battelle, LLC under Contract no.
DE-AC05-00OR22725 with the U.S. Department of Energy.
NR 10
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SN 0168-9002
EI 1872-9576
J9 NUCL INSTRUM METH A
JI Nucl. Instrum. Methods Phys. Res. Sect. A-Accel. Spectrom. Dect. Assoc.
Equip.
PD OCT 11
PY 2016
VL 833
BP 38
EP 44
DI 10.1016/j.nima.2016.06.112
PG 7
WC Instruments & Instrumentation; Nuclear Science & Technology; Physics,
Nuclear; Physics, Particles & Fields
SC Instruments & Instrumentation; Nuclear Science & Technology; Physics
GA DW7GC
UT WOS:000383818200007
ER
PT J
AU Huang, TC
Ma, R
Huang, B
Huang, X
Ruan, L
Todoroki, T
Xu, Z
Yang, C
Yang, S
Yang, Q
Yang, Y
Zha, W
AF Huang, T. C.
Ma, R.
Huang, B.
Huang, X.
Ruan, L.
Todoroki, T.
Xu, Z.
Yang, C.
Yang, S.
Yang, Q.
Yang, Y.
Zha, W.
TI Muon identification with Muon Telescope Detector at the STAR experiment
SO NUCLEAR INSTRUMENTS & METHODS IN PHYSICS RESEARCH SECTION A-ACCELERATORS
SPECTROMETERS DETECTORS AND ASSOCIATED EQUIPMENT
LA English
DT Article
DE STAR; MTD; Muon identification; Muon; Dimuon; Quarkonium
AB The Muon Telescope Detector (MID) is a newly installed detector in the STAR experiment. It provides an excellent opportunity to study heavy quarkonium physics using the dimuon channel in heavy ion collisions. In this paper, we report the muon identification performance for the MTD using proton-proton collisions at root s =500 GeV with various methods. The result using the Likelihood Ratio method shows that the muon identification efficiency can reach up to similar to 90% for muons with transverse momenta greater than 3 GeV/c and the significance of the J/psi signal is improved by a factor of 2 compared to using the basic selection. (C) 2016 Elsevier B.V. All rights reserved.
C1 [Huang, T. C.; Yang, Y.] Natl Cheng Kung Univ, Tainan 70101, Taiwan.
[Ma, R.; Ruan, L.; Todoroki, T.; Xu, Z.] Brookhaven Natl Lab, Upton, NY 11973 USA.
[Huang, X.] Tsinghua Univ, Beijing 100084, Peoples R China.
[Huang, B.] Univ Illinois, Chicago, IL 60607 USA.
[Yang, C.; Yang, S.; Yang, Q.; Zha, W.] Univ Sci & Technol China, Hefei 230026, Peoples R China.
RP Yang, Y (reprint author), Natl Cheng Kung Univ, Tainan 70101, Taiwan.
EM yiyang@ncku.edu.tw
FU STAR Collaboration; RACF at BNL; National Cheng Kung University
(Taiwan); U.S. DOE Office of Science [de-sc0012704]; Goldhaber
Fellowship program at Brookhaven National Laboratory
FX We thank the STAR Collaboration, the RACF at BNL and National Cheng Kung
University (Taiwan) for their support. This work was supported in part
by the U.S. DOE Office of Science under the Contract no. de-sc0012704
and the Goldhaber Fellowship program at Brookhaven National Laboratory.
L. Ruan acknowledges a DOE Office of Science Early Career Award. We
thank Dr. Gene Van Buren (BNL) for the proofreading.
NR 13
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SN 0168-9002
EI 1872-9576
J9 NUCL INSTRUM METH A
JI Nucl. Instrum. Methods Phys. Res. Sect. A-Accel. Spectrom. Dect. Assoc.
Equip.
PD OCT 11
PY 2016
VL 833
BP 88
EP 93
DI 10.1016/j.nima.2016.07.024
PG 6
WC Instruments & Instrumentation; Nuclear Science & Technology; Physics,
Nuclear; Physics, Particles & Fields
SC Instruments & Instrumentation; Nuclear Science & Technology; Physics
GA DW7GC
UT WOS:000383818200015
ER
PT J
AU Sweany, M
Marleau, P
AF Sweany, M.
Marleau, P.
TI Design and expected performance of a fast neutron attenuation probe for
light element density measurements
SO NUCLEAR INSTRUMENTS & METHODS IN PHYSICS RESEARCH SECTION A-ACCELERATORS
SPECTROMETERS DETECTORS AND ASSOCIATED EQUIPMENT
LA English
DT Article
DE Neutron time-of-flight; Material identification; Explosives detection
ID RADIOGRAPHY; SYSTEM
AB We present the design and expected performance of a proof-of-concept 32 channel material identification system. Our system is based on the energy-dependent attenuation of fast neutrons for four elements: hydrogen, carbon, nitrogen and oxygen. We describe a new approach to obtaining a broad range of neutron energies to probe a sample, as well as our technique for reconstructing the molar densities within a sample. The system's performance as a function of time-of-flight energy resolution is explored using a Geant4-based Monte Carlo. Our results indicate that, with the expected detector response of our system, we will be able to determine the molar density of all four elements to within a 20-30% accuracy in a two hour scan time. In many cases this error is systematically low, thus the ratio between elements is more accurate. This degree of accuracy is enough to distinguish, for example, a sample of water from a sample of pure hydrogen peroxide: the ratio of oxygen to hydrogen is reconstructed to within 8 +/- 0.5% of the true value. Finally, with future algorithm development that accounts for backgrounds caused by scattering within the sample itself, the accuracy of molar densities, not ratios, may improve to the 5-10% level for a two hour scan time. (C) 2016 Elsevier B.V. All rights reserved.
C1 [Sweany, M.; Marleau, P.] Sandia Natl Labs, Livermore, CA 94550 USA.
RP Sweany, M (reprint author), Sandia Natl Labs, Livermore, CA 94550 USA.
EM msweany@sandia.gov
FU Laboratory Directed Research and Development (LDRD) at Sandia National
Laboratories; U.S. Department of Energy's National Nuclear Security
Administration [DE-AC04-94AL85000]
FX This work was supported by Laboratory Directed Research and Development
(LDRD) at Sandia National Laboratories. Sandia National Laboratories is
a multi-program laboratory managed and operated by Sandia Corporation, a
wholly owned subsidiary of Lockheed Martin Corporation, for the U.S.
Department of Energy's National Nuclear Security Administration under
contract DE-AC04-94AL85000. Document release number SAND2016-6250 J.
NR 12
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SN 0168-9002
EI 1872-9576
J9 NUCL INSTRUM METH A
JI Nucl. Instrum. Methods Phys. Res. Sect. A-Accel. Spectrom. Dect. Assoc.
Equip.
PD OCT 11
PY 2016
VL 833
BP 134
EP 141
DI 10.1016/j.nima.2016.07.011
PG 8
WC Instruments & Instrumentation; Nuclear Science & Technology; Physics,
Nuclear; Physics, Particles & Fields
SC Instruments & Instrumentation; Nuclear Science & Technology; Physics
GA DW7GC
UT WOS:000383818200021
ER
PT J
AU Herrera, E
Hamm, D
Wiggins, B
Milburn, R
Burger, A
Bilheux, H
Santodonato, L
Chvala, O
Stowe, A
Lukosi, E
AF Herrera, Elan
Hamm, Daniel
Wiggins, Brenden
Milburn, Rob
Burger, Arnold
Bilheux, Hassina
Santodonato, Louis
Chvala, Ondrej
Stowe, Ashley
Lukosi, Eric
TI LISe pixel detector for neutron imaging
SO NUCLEAR INSTRUMENTS & METHODS IN PHYSICS RESEARCH SECTION A-ACCELERATORS
SPECTROMETERS DETECTORS AND ASSOCIATED EQUIPMENT
LA English
DT Article
DE (LiInSe2)-Li-6; LISe; Neutron detection; Neutron imaging; Pixel
detector; Semiconductor detector
ID FLUX ISOTOPE REACTOR; CHIP
AB Semiconducting lithium indium diselenide, (LiInSe2)-Li-6 or LISe, has promising characteristics for neutron detection applications. The 95% isotopic enrichment of Li-6 results in a highly efficient thermal neutron sensitive material. In this study, we report on a proof-of-principle investigation of a semiconducting LISe pixel detector to demonstrate its potential as an efficient neutron imager. The LISe pixel detector had a 4 x 4 of pixels with a 550 mu m pitch on a 5 x 5 x 0.56 mm(3) LISe substrate. An experimentally verified spatial resolution of 300 mu m was observed utilizing a super-sampling technique. (C) 2016 Elsevier B.V. All rights reserved.
C1 [Herrera, Elan; Hamm, Daniel; Milburn, Rob; Chvala, Ondrej; Stowe, Ashley; Lukosi, Eric] Univ Tennessee, Dept Nucl Engn, Knoxville, TN 37996 USA.
[Wiggins, Brenden; Stowe, Ashley] Technol Dev, Y-12 Natl Secur Complex, Oak Ridge, TN USA.
[Wiggins, Brenden] Vanderbilt Univ, Dept Phys & Astron, Nashville, TN 37235 USA.
[Burger, Arnold] Fisk Univ, Dept Life & Phys Sci, Nashville, TN USA.
[Bilheux, Hassina] Oak Ridge Natl Lab, Chem & Engn Mat Div, Oak Ridge, TN USA.
[Santodonato, Louis] Oak Ridge Natl Lab, Instrument & Source Div, Oak Ridge, TN USA.
RP Lukosi, E (reprint author), Univ Tennessee, Dept Nucl Engn, Knoxville, TN 37996 USA.
EM elukosi@utk.edu
RI Santodonato, Louis/A-9523-2015; Bilheux, Hassina/H-4289-2012
OI Santodonato, Louis/0000-0002-4600-685X; Bilheux,
Hassina/0000-0001-8574-2449
FU CNS Y-12 National Security Complex [4300090406]; Department of Energy
Nuclear Energy University Programs Graduate Fellowship [DE-NE0000094];
Scientific User Facilities Division, Office of Basic Energy Sciences,
U.S. Department of Energy
FX This work is supported through subcontract number 4300090406 from CNS
Y-12 National Security Complex and under a Department of Energy Nuclear
Energy University Programs Graduate Fellowship (DE-NE0000094). A portion
of this research at ORNL's High Flux Isotope Reactor was sponsored by
the Scientific User Facilities Division, Office of Basic Energy
Sciences, U.S. Department of Energy.
NR 26
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PI AMSTERDAM
PA PO BOX 211, 1000 AE AMSTERDAM, NETHERLANDS
SN 0168-9002
EI 1872-9576
J9 NUCL INSTRUM METH A
JI Nucl. Instrum. Methods Phys. Res. Sect. A-Accel. Spectrom. Dect. Assoc.
Equip.
PD OCT 11
PY 2016
VL 833
BP 142
EP 148
DI 10.1016/j.nima.2016.07.035
PG 7
WC Instruments & Instrumentation; Nuclear Science & Technology; Physics,
Nuclear; Physics, Particles & Fields
SC Instruments & Instrumentation; Nuclear Science & Technology; Physics
GA DW7GC
UT WOS:000383818200022
ER
PT J
AU Masui, H
Schmah, A
Poskanzer, AM
AF Masui, Hiroshi
Schmah, Alexander
Poskanzer, A. M.
TI Event plane resolution correction for azimuthal anisotropy in wide
centrality bins
SO NUCLEAR INSTRUMENTS & METHODS IN PHYSICS RESEARCH SECTION A-ACCELERATORS
SPECTROMETERS DETECTORS AND ASSOCIATED EQUIPMENT
LA English
DT Article
DE Azimuthal anisotropy; Flow; Event plane resolution
ID RELATIVISTIC NUCLEAR COLLISIONS; FLOW
AB We provide a method to correct the observed azimuthal anisotropy in heavy-ion collisions for the event plane resolution in a wide centrality bin. This new procedure is especially useful for rare particles, such as Omega baryons and J/psi mesons, which are difficult to measure in small intervals of centrality. Based on a Monte Carlo calculation with simulated v(2) and multiplicity, we show that some of the commonly used methods have a bias of up to 15%. (C) 2016 Elsevier B.V. All rights reserved.
C1 [Masui, Hiroshi; Schmah, Alexander; Poskanzer, A. M.] Lawrence Berkeley Natl Lab, Berkeley, CA 94720 USA.
RP Poskanzer, AM (reprint author), Lawrence Berkeley Natl Lab, Berkeley, CA 94720 USA.
EM hirmasui@gmail.com; ASchmah@lbl.gov; AMPoskanzer@lbl.gov
FU US Department of Energy [DE-AC03-76SF00098]
FX We thank Jean-Yves Ollitrault, Shusu Shi, and Xu Sun for discussions.
This paper was funded in part by the US Department of Energy under
Contract No. DE-AC03-76SF00098.
NR 11
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U1 0
U2 0
PU ELSEVIER SCIENCE BV
PI AMSTERDAM
PA PO BOX 211, 1000 AE AMSTERDAM, NETHERLANDS
SN 0168-9002
EI 1872-9576
J9 NUCL INSTRUM METH A
JI Nucl. Instrum. Methods Phys. Res. Sect. A-Accel. Spectrom. Dect. Assoc.
Equip.
PD OCT 11
PY 2016
VL 833
BP 181
EP 185
DI 10.1016/j.nima.2016.07.037
PG 5
WC Instruments & Instrumentation; Nuclear Science & Technology; Physics,
Nuclear; Physics, Particles & Fields
SC Instruments & Instrumentation; Nuclear Science & Technology; Physics
GA DW7GC
UT WOS:000383818200027
ER
PT J
AU Vaccaro, S
Tobin, SJ
Favalli, A
Grogan, B
Jansson, P
Liljenfeldt, H
Mozin, V
Hu, J
Schwalbach, P
Sjoland, A
Trellue, H
Vo, D
AF Vaccaro, S.
Tobin, S. J.
Favalli, A.
Grogan, B.
Jansson, P.
Liljenfeldt, H.
Mozin, V.
Hu, J.
Schwalbach, P.
Sjoland, A.
Trellue, H.
Vo, D.
TI PWR and BWR spent fuel assembly gamma spectra measurements
SO NUCLEAR INSTRUMENTS & METHODS IN PHYSICS RESEARCH SECTION A-ACCELERATORS
SPECTROMETERS DETECTORS AND ASSOCIATED EQUIPMENT
LA English
DT Article
DE Passive gamma; Bumup; Cooling time; Gamma spectroscopy; Spent fuel;
Nuclear safeguards; Germanium detector; Final disposal; Non-destructive
assay
AB A project to research the application of nondestructive assay (NDA) to spent fuel assemblies is underway. The research team comprises the European Atomic Energy Community (EURATOM), embodied by the European Commission, DG Energy, Directorate EURATOM Safeguards; the Swedish Nuclear Fuel and Waste Management Company (SKB); two universities; and several United States national laboratories. The Next Generation of Safeguards Initiative-Spent Fuel project team is working to achieve the following technical goals more easily and efficiently than in the past using nondestructive assay measurements of spent fuel assemblies: (1) verify the initial enrichment, burnup, and cooling time of facility declaration; (2) detect the diversion or replacement of pins, (3) estimate the plutonium mass, (4) estimate the decay heat, and (5) determine the reactivity of spent fuel assemblies. This study focuses on spectrally resolved gamma-ray measurements performed on a diverse set of 50 assemblies [25 pressurized water reactor (PWR) assemblies and 25 boiling water reactor (BWR) assemblies]; these same 50 assemblies will be measured with neutron-based NDA instruments and a full-length calorimeter. Given that encapsulation/repository and dry storage safeguards are the primarily intended applications, the analysis focused on the dominant gamma-ray lines of Cs-137, Eu-154, and Cs-134 because these isotopes will be the primary gamma ray emitters during the time frames of interest to these applications. This study addresses the impact on "the measured passive gamma-ray signals due to the following factors: burnup, initial enrichment, cooling time, assembly type (eight different PWR and six different BWR fuel designs), presence of gadolinium rods, and anomalies in operating history. To compare the measured results with theory, a limited number of ORIGEN-ARP simulations were performed. (C) 2016 Elsevier B.V. All rights reserved.
C1 [Vaccaro, S.; Schwalbach, P.] European Commiss, DG Energy, Directorate EURATOM Safeguards Luxembourg, Luxembourg, Luxembourg.
[Tobin, S. J.; Favalli, A.; Trellue, H.; Vo, D.] Los Alamos Natl Lab, Los Alamos, NM USA.
[Grogan, B.; Liljenfeldt, H.; Hu, J.] Oak Ridge Natl Lab, Oak Ridge, TN USA.
[Jansson, P.] Uppsala Univ, Uppsala, Sweden.
[Liljenfeldt, H.; Sjoland, A.] Swedish Nucl Fuel & Waste Management Co SKB, Stockholm, Sweden.
[Mozin, V.] Lawrence Livermore Natl Lab, Livermore, CA USA.
RP Vaccaro, S (reprint author), European Commiss, DG Energy, Directorate EURATOM Safeguards Luxembourg, Luxembourg, Luxembourg.
NR 24
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PI AMSTERDAM
PA PO BOX 211, 1000 AE AMSTERDAM, NETHERLANDS
SN 0168-9002
EI 1872-9576
J9 NUCL INSTRUM METH A
JI Nucl. Instrum. Methods Phys. Res. Sect. A-Accel. Spectrom. Dect. Assoc.
Equip.
PD OCT 11
PY 2016
VL 833
BP 208
EP 225
DI 10.1016/j.nima.2016.07.032
PG 18
WC Instruments & Instrumentation; Nuclear Science & Technology; Physics,
Nuclear; Physics, Particles & Fields
SC Instruments & Instrumentation; Nuclear Science & Technology; Physics
GA DW7GC
UT WOS:000383818200031
ER
PT J
AU Kong, XL
Chen, Y
Feng, SW
Du, GH
Li, CY
Koval, A
Vasanth, V
Wang, B
Guo, F
Li, G
AF Kong, Xiangliang
Chen, Yao
Feng, Shiwei
Du, Guohui
Li, Chuanyang
Koval, Artem
Vasanth, V.
Wang, Bing
Guo, Fan
Li, Gang
TI OBSERVATION OF A METRIC TYPE N SOLAR RADIO BURST
SO ASTROPHYSICAL JOURNAL
LA English
DT Article
DE Sun: corona; Sun: flares; Sun: magnetic fields; Sun: radio radiation
ID CORONAL MAGNETIC-FIELDS; ELECTRON-BEAMS; III BURSTS;
PARTICLE-ACCELERATION; HARMONIC EMISSION; U-BURSTS; POLARIZATION;
FREQUENCY; PLASMA; INTERPLANETARY
AB Type III and type-III-like radio bursts are produced by energetic electron beams guided along coronal magnetic fields. As a variant of type III bursts, Type N bursts appear as the letter "N" in the radio dynamic spectrum and reveal a magnetic mirror effect in coronal loops. Here, we report a well-observed N-shaped burst consisting of three successive branches at metric wavelength with both fundamental and harmonic components and a high brightness temperature (>10(9) K). We verify the burst as a true type N burst generated by the same electron beam from three aspects of the data. First, durations of the three branches at a given frequency increase gradually and. may be. due to the dispersion of the beam along its path. Second, the flare site, as the only possible source of non-thermal electrons, is near the western feet of large-scale closed loops. Third, the first branch and the following two branches are localized at different legs of the loops with opposite senses of. polarization. We also find that the sense of polarization of the radio burst is in contradiction to the O-mode and there exists a fairly large time delay (similar to 3-5 s) between the fundamental and harmonic components. Possible explanations accounting for these observations are presented. Assuming the classical plasma emission mechanism, we can infer coronal parameters such as electron density and magnetic field near the radio source and make diagnostics on the magnetic mirror process.
C1 [Kong, Xiangliang; Chen, Yao; Feng, Shiwei; Du, Guohui; Li, Chuanyang; Koval, Artem; Vasanth, V.; Wang, Bing] Shandong Univ, Shandong Prov Key Lab Opt Astron & Solar Terr Env, Weihai 264209, Shandong, Peoples R China.
[Kong, Xiangliang; Chen, Yao; Feng, Shiwei; Du, Guohui; Li, Chuanyang; Koval, Artem; Vasanth, V.; Wang, Bing] Shandong Univ, Inst Space Sci, Weihai 264209, Shandong, Peoples R China.
[Koval, Artem] Natl Acad Sci Ukraine, Inst Radio Astron, UA-61002 Kharkov, Ukraine.
[Guo, Fan] Los Alamos Natl Lab, Div Theoret, Los Alamos, NM 87545 USA.
[Li, Gang] Univ Alabama, Dept Space Sci, Huntsville, AL 35899 USA.
[Li, Gang] Univ Alabama, CSPAR, Huntsville, AL 35899 USA.
RP Kong, XL (reprint author), Shandong Univ, Shandong Prov Key Lab Opt Astron & Solar Terr Env, Weihai 264209, Shandong, Peoples R China.; Kong, XL (reprint author), Shandong Univ, Inst Space Sci, Weihai 264209, Shandong, Peoples R China.
EM kongx@sdu.edu.cn
RI V, Vasanth/N-1056-2014; Chen, Yao/B-7255-2011; Kong,
Xiangliang/D-9855-2012;
OI Koval, Artem/0000-0002-1732-1738
FU Natural Science Foundation of Shandong Province [ZR2014DQ001]; NSF
[ATM-0847719, AGS1135432]; NSBRSF [2012CB825601]; NNSFC [11503014,
41274175, 41331068, U1431103]
FX We thank the teams of e-Callisto, ORFEES, NRH, DAM, IZMIRAN, RSTN,
SDO/AIA, and SDO/HMI for making their data available to us. This work
was supported by grants NSBRSF 2012CB825601, NNSFC 11503014, 41274175,
41331068, U1431103, and Natural Science Foundation of Shandong Province
ZR2014DQ001. Gang Li's work at UAHuntsville was supported by NSF grants
ATM-0847719 and AGS1135432.
NR 61
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U1 2
U2 2
PU IOP PUBLISHING LTD
PI BRISTOL
PA TEMPLE CIRCUS, TEMPLE WAY, BRISTOL BS1 6BE, ENGLAND
SN 0004-637X
EI 1538-4357
J9 ASTROPHYS J
JI Astrophys. J.
PD OCT 10
PY 2016
VL 830
IS 1
AR 37
DI 10.3847/0004-637X/830/1/37
PG 7
WC Astronomy & Astrophysics
SC Astronomy & Astrophysics
GA EM4ME
UT WOS:000395286300001
ER
PT J
AU Li, HB
Wu, KF
Lim, J
Song, HJ
Klimov, VI
AF Li, Hongbo
Wu, Kaifeng
Lim, Jaehoon
Song, Hyung-Jun
Klimov, Victor I.
TI Doctor-blade deposition of quantum dots onto standard window glass for
low-loss large-area luminescent solar concentrators
SO NATURE ENERGY
LA English
DT Article
ID CORE-SHELL INTERFACE; SEMICONDUCTOR NANOCRYSTALS; AUGER RECOMBINATION;
SILICA SPHERES; STOKES-SHIFT; DEVICES; BRIGHT; ENERGY; PERFORMANCE;
EFFICIENCY
AB Luminescent solar concentrators (LSCs) are envisioned to reduce the cost of solar electricity by decreasing the usage of more expensive photovoltaic (PV) materials and diminishing the complexity of multi-cell PV modules. The LSC concept can also enable unconventional solar-energy conversion devices such as PV windows that can be especially useful in highly populated urban areas. Here we demonstrate low-loss, large-area (up to about 90 x 30 cm(2)) LSCs fabricated from colloidal core/shell quantum dots (QDs) whose optical spectra are tailored so as to minimize self-absorption of waveguided radiation. For improved compatibility with a polymer matrix and enhanced stability, QDs are encapsulated into silica shells, which allows for maintaining high emission efficiencies (similar to 70% quantum yields) under four-month exposure to air and light, and heat treatments up to 200 degrees C. The QD/polymer composites are processed into devices using standard doctor-blade deposition onto commercial window glasses. The fabricated semi-transparent devices demonstrate internal quantum efficiencies of more than 10% for dimensions of tens of centimetres.
C1 [Li, Hongbo; Wu, Kaifeng; Lim, Jaehoon; Song, Hyung-Jun; Klimov, Victor I.] Los Alamos Natl Lab, Div Chem, Ctr Adv Solar Photophys, Los Alamos, NM 87545 USA.
RP Klimov, VI (reprint author), Los Alamos Natl Lab, Div Chem, Ctr Adv Solar Photophys, Los Alamos, NM 87545 USA.
EM klimov@lanl.gov
FU Centre for Advanced Solar Photophysics (CASP), an Energy Frontier
Research Centre - the US Department of Energy, Office of Science, Basic
Energy Sciences
FX This work was supported by the Centre for Advanced Solar Photophysics
(CASP), an Energy Frontier Research Centre funded by the US Department
of Energy, Office of Science, Basic Energy Sciences. The authors would
like to thank N. S. Makarov for assistance in setting up a system for
accelerated photostability tests.
NR 43
TC 2
Z9 2
U1 7
U2 7
PU NATURE PUBLISHING GROUP
PI LONDON
PA MACMILLAN BUILDING, 4 CRINAN ST, LONDON N1 9XW, ENGLAND
SN 2058-7546
J9 NAT ENERGY
JI Nat. Energy
PD OCT 10
PY 2016
VL 1
AR 16157
DI 10.1038/NENERGY.2016.157
PG 9
WC Energy & Fuels; Materials Science, Multidisciplinary
SC Energy & Fuels; Materials Science
GA EL7HF
UT WOS:000394791000001
ER
PT J
AU Fisher, MK
Argall, MR
Joyce, CJ
Smith, CW
Isenberg, PA
Vasquez, BJ
Schwadron, NA
Skoug, RM
Sokol, JM
Bzowski, M
Zurbuchen, TH
Gilbert, JA
AF Fisher, Meghan K.
Argall, Matthew R.
Joyce, Colin J.
Smith, Charles W.
Isenberg, Philip A.
Vasquez, Bernard J.
Schwadron, Nathan A.
Skoug, Ruth M.
Sokol, Justyna M.
Bzowski, Maciej
Zurbuchen, Thomas H.
Gilbert, Jason A.
TI A SURVEY OF MAGNETIC WAVES EXCITED BY NEWBORN INTERSTELLAR He+ OBSERVED
BY THE ACE SPACECRAFT AT 1 au
SO ASTROPHYSICAL JOURNAL
LA English
DT Article
DE instabilities; magnetic fields; solar wind; Sun: heliosphere;
turbulence; waves
ID SOLAR-WIND TURBULENCE; ADVANCED COMPOSITION EXPLORER; ROTATING
RAREFACTION REGIONS; PICKUP IONS; MAGNETOHYDRODYNAMIC TURBULENCE;
DISSIPATION RANGE; NEUTRAL HELIUM; STATISTICAL-ANALYSIS; ULYSSES
OBSERVATIONS; VOYAGER OBSERVATIONS
AB We report observations of low-frequency waves at 1 au by the magnetic field instrument on the Advanced Composition Explorer (ACE/MAG) and show evidence that they arise due to newborn interstellar pickup He+. Twenty-five events are studied. They possess the generally predicted attributes: spacecraft-frame frequencies slightly greater than the He+ cyclotron frequency, left-hand polarization in the spacecraft frame, and transverse fluctuations with minimum variance directions that are quasi-parallel to the mean magnetic field. Their occurrence spans the first 18 years of ACE operations, with no more than 3 such observations in any given year. Thus, the events are relatively rare. As with past observations by the Ulysses and Voyager spacecraft, we argue that the waves are seen only when the background turbulence is sufficiently weak as to allow for the slow accumulation of wave energy over many hours.
C1 [Fisher, Meghan K.; Argall, Matthew R.; Joyce, Colin J.; Smith, Charles W.; Isenberg, Philip A.; Vasquez, Bernard J.; Schwadron, Nathan A.] Univ New Hampshire, Dept Phys, Morse Hall, Durham, NH 03824 USA.
[Fisher, Meghan K.; Argall, Matthew R.; Joyce, Colin J.; Smith, Charles W.; Isenberg, Philip A.; Vasquez, Bernard J.; Schwadron, Nathan A.] Univ New Hampshire, Ctr Space Sci, Morse Hall, Durham, NH 03824 USA.
[Skoug, Ruth M.] Los Alamos Natl Lab, Space & Atmospher Sci, Los Alamos, NM USA.
[Sokol, Justyna M.; Bzowski, Maciej] Polish Acad Sci, CBK PAN, Space Res Ctr, Bartycka 18A, Warsaw, Poland.
[Zurbuchen, Thomas H.; Gilbert, Jason A.] Univ Michigan, Dept Climate & Space Sci & Engn, Ann Arbor, MI 48109 USA.
RP Fisher, MK (reprint author), Univ New Hampshire, Dept Phys, Morse Hall, Durham, NH 03824 USA.; Fisher, MK (reprint author), Univ New Hampshire, Ctr Space Sci, Morse Hall, Durham, NH 03824 USA.
EM mkl54@wildcats.unh.edu; Matthew.Argall@unh.edu; cjl46@wildcats.unh.edu;
Charles.Smith@unh.edu; Phil.Isenberg@unh.edu; Bernie.Vasquez@unh.edu;
Nathan.Schwadron@unh.edu; rskoug@lanl.gov; jsokol@cbk.waw.pl;
bzowski@cbk.waw.pl; thomasz@umich.edu; jagi@umich.edu
RI Sokol, Justyna/K-2892-2015
FU Caltech subcontract [44A1085631]; NASA [NNX13AF97G, NNX13AH66G]; NSF
SHINE grant [AGS1358103, AGS1357893]; Polish National Science Center
grant [2015/18/M/ST9/00036]
FX Unsmoothed monthly sunspot numbers were obtained from NOAA at
ftp://ftp.ngdc.noaa.gov/STP/. C.W.S. and M.K.F. are supported by Caltech
subcontract 44A1085631 to the University of New Hampshire in support of
the ACE/MAG instrument. P.A.I. is supported by NASA grant NNX13AF97G and
by an NSF SHINE grant AGS1358103. B.J.V. is supported by NSF/SHINE grant
AGS1357893. J.M.S. and M.B. acknowledge the support by the Polish
National Science Center grant 2015/18/M/ST9/00036. T.H.Z. and J.A.G. are
supported, in part, by NASA grant NNX13AH66G. M.K.F. is an undergraduate
physics major at UNH. C.J.J. is a graduate student completing his Ph.D.
in physics at UNH. M.R.A. is a recent Ph.D. from the UNH program.
NR 117
TC 0
Z9 0
U1 2
U2 2
PU IOP PUBLISHING LTD
PI BRISTOL
PA TEMPLE CIRCUS, TEMPLE WAY, BRISTOL BS1 6BE, ENGLAND
SN 0004-637X
EI 1538-4357
J9 ASTROPHYS J
JI Astrophys. J.
PD OCT 10
PY 2016
VL 830
IS 1
AR 47
DI 10.3847/0004-637X/830/1/47
PG 14
WC Astronomy & Astrophysics
SC Astronomy & Astrophysics
GA EK0NK
UT WOS:000393623200001
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CA CMS Collaboration
TI Upsilon (nS) polarizations versus particle multiplicity in pp collisions
at root s=7 TeV
SO PHYSICS LETTERS B
LA English
DT Article
DE CMS; Physics; Quarkonium production; Quarkonium polarization; QCD medium
effects
ID QUARKONIUM
AB The polarizations of the Upsilon(1S), Upsilon(2S), and Upsilon(3S) mesons are measured as a function of the charged particle multiplicity in proton-proton collisions at root s = 7 TeV. The measurements are performed with a dimuon data sample collected in 2011 by the CMS experiment, corresponding to an integrated luminosity of 4.9fb(-1). The results are extracted from the dimuon decay angular distributions, in two ranges of Upsilon(nS) transverse momentum (10-15 and 15-35 GeV), and in the rapidity interval |y| < 1.2. The results do not show significant changes from low-to high-multiplicity pp collisions, although large uncertainties preclude definite statements in the Upsilon(2S) and Upsilon(3S) cases. (C) 2016 The Author(s). Published by Elsevier B.V.
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[Adam, W.; Asilar, E.; Bergauer, T.; Brandstetter, J.; Brondolin, E.; Dragicevic, M.; Ero, J.; Fabjan, C.; Flechl, M.; Friedl, M.; Fruhwirth, R.; Ghete, V. M.; Hartl, C.; Hormann, N.; Hrubec, J.; Jeitler, M.; Knunz, V.; Konig, A.; Krammer, M.; Kratschmer, I.; Liko, D.; Matsushita, T.; Mikulec, I.; Rabady, D.; Rad, N.; Rahbaran, B.; Rohringer, H.; Schieck, J.; Schofbeck, R.; Strauss, J.; Treberer-Treberspurg, W.; Waltenberger, W.; Wulz, C. -E.] Inst Hochenergiephys OeAW, Vienna, Austria.
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[Beernaert, K.; Benucci, L.; Cimmino, A.; Crucy, S.; Dobur, D.; Fagot, A.; Garcia, G.; Gul, M.; Mccartin, J.; Poyraz, D.; Ryckbosch, D.; Salva, S.; Sigamani, M.; Tytgat, M.; Van Driessche, W.; Yazgan, E.; Zaganidis, N.] Univ Ghent, Ghent, Belgium.
[Basegmez, S.; Beluffi, C.; Bondu, O.; Brochet, S.; Bruno, G.; Caudron, A.; Ceard, L.; Delaere, C.; Favart, D.; Forthomme, L.; Giammanco, A.; Jafari, A.; Jez, P.; Komm, M.; Lemaitre, V.; Mertens, A.; Musich, M.; Nuttens, C.; Perrini, L.; Piotrzkowski, K.; Popov, A.; Quertenmont, L.; Selvaggi, M.; Marono, M. Vidal] Catholic Univ Louvain, Louvain La Neuve, Belgium.
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[Zhang, F.; Asawatangtrakuldee, C.; Ban, Y.; Li, Q.; Liu, S.; Mao, Y.; Qian, S. J.; Wang, D.; Xu, Z.; Romanowska-Rybinska, K.] Peking Univ, State Key Lab Nucl Phys & Technol, Beijing, Peoples R China.
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[Brigljevic, V.; Kadija, K.; Luetic, J.; Micanovic, S.; Sudic, L.] Inst Rudjer Boskov, Zagreb, Croatia.
[Attikis, A.; Mavromanolakis, G.; Mousa, J.; Nicolaou, C.; Ptochos, F.; Razis, P. A.; Rykaczewski, H.] Univ Cyprus, Nicosia, Cyprus.
[Bodlak, M.; Finger, M.; Finger, M., Jr.] Charles Univ Prague, Prague, Czech Republic.
[Abdelalim, A. A.; Awad, A.; Mahrous, A.; Radi, A.] Egyptian Network High Energy Phys, Acad Sci Res & Technol Arab Republ Egypt, Cairo, Egypt.
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[Eerola, P.; Pekkanen, J.; Voutilainen, M.] Univ Helsinki, Dept Phys, Helsinki, Finland.
[Harkonen, J.; Karimaki, V.; Kinnunen, R.; Lampen, T.; Lassila-Perini, K.; Lehti, S.; Linden, T.; Luukka, P.; Peltola, T.; Tuominiemi, J.; Tuovinen, E.; Wendland, L.] Helsinki Inst Phys, Helsinki, Finland.
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[Plestina, R.; Abdulsalam, A.; Antropov, I.; Baffioni, S.; Beaudette, F.; Busson, P.; Cadamuro, L.; Chapon, E.; Chariot, C.; Davignon, O.; Filipovic, N.; de Cassagnac, R. Granier; Jo, M.; Lisniak, S.; Mastrolorenzo, L.; Mine, P.; Naranjo, I. N.; Nguyen, M.; Ochando, C.; Ortona, G.; Paganini, P.; Pigard, P.; Regnard, S.; Salerno, R.; Sauvan, J. B.; Sirois, Y.; Strebler, T.; Yilmaz, Y.; Zabi, A.] Ecole Polytech, Lab Leprince Ringuet, IN2P3 CNRS, Palaiseau, France.
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[Toriashvili, T.; Tsamalaidze, Z.] Tbilisi State Univ, Tbilisi, Rep of Georgia.
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[Cherepanov, V.; Erdogan, Y.; Flugge, G.; Geenen, H.; Geisler, M.; Hoehle, F.; Kargoll, B.; Kress, T.; Kunsken, A.; Lingemann, J.; Nehrkorn, A.; Nowack, A.; Nugent, I. M.; Pistone, C.; Pooth, O.; Stahl, A.] Rhein Westfal TH Aachen, Phys Inst B 3, Aachen, Germany.
[Martin, M. Aldaya; Asin, I.; Bartosik, N.; Behnke, O.; Behrens, U.; Borras, K.; Burgmeier, A.; Campbell, A.; Contreras-Campana, C.; Costanza, F.; Pardos, C. Diez; Dolinska, G.; Dooling, S.; Dorland, T.; Eckerlin, G.; Eckstein, D.; Eichhorn, T.; Flucke, G.; Gallo, E.; Garcia, J. Garay; Geiser, A.; Gizhko, A.; Gunnellini, P.; Hauk, J.; Hempel, M.; Jung, H.; Kalogeropoulos, A.; Karacheban, O.; Kasemann, M.; Katsas, P.; Kieseler, J.; Kleinwort, C.; Korol, I.; Lange, W.; Leonard, J.; Lipka, K.; Lobanov, A.; Lohmann, W.; Mankel, R.; Melzer-Pellmann, I. -A.; Meyer, A. B.; Mittag, G.; Mnich, J.; Mussgiller, A.; Naumann-Emme, S.; Nayak, A.; Ntomari, E.; Perrey, H.; Pitzl, D.; Placakyte, R.; Raspereza, A.; Roland, B.; Sahin, M. O.; Saxena, P.; Schoerner-Sadenius, T.; Seitz, C.; Spannagel, S.; Stefaniuk, N.; Trippkewitz, K. D.; Walsh, R.; Wissing, C.] DESY, Hamburg, Germany.
[Gallo, E.; Blobel, V.; Vignali, M. Centis; Draeger, A. R.; Erfle, J.; Garutti, E.; Goebel, K.; Gonzalez, D.; Gorner, M.; Haller, J.; Hoffmann, M.; Hoing, R. S.; Junkes, A.; Klanner, R.; Kogler, R.; Kovalchuk, N.; Lapsien, T.; Lenz, T.; Marchesini, I.; Marconi, D.; Meyer, M.; Nowatschin, D.; Ott, J.; Pantaleo, F.; Peiffer, T.; Perieanu, A.; Pietsch, N.; Poehlsen, J.; Rathjens, D.; Sander, C.; Scharf, C.; Schleper, P.; Schlieckau, E.; Schmidt, A.; Schumann, S.; Schwandt, J.; Sola, V.; Stadie, H.; Steinbruck, G.; Stober, F. M.; Tholen, H.; Troendle, D.; Usai, E.; Vanelderen, L.; Vanhoefer, A.; Vormwald, B.] Univ Hamburg, Hamburg, Germany.
[Barth, C.; Baus, C.; Berger, J.; Boser, C.; Butz, E.; Chwalek, T.; Colombo, F.; De Boer, W.; Descroix, A.; Dierlamm, A.; Fink, S.; Frensch, F.; Friese, R.; Giffels, M.; Gilbert, A.; Haitz, D.; Hartmann, F.; Heindl, S. M.; Husemann, U.; Katkov, I.; Kornmayer, A.; Pardo, P. Lobelle; Maier, B.; Mildner, H.; Mozer, M. U.; Muller, T.; Muller, Th.; Plagge, M.; Quast, G.; Rabbertz, K.; Rocker, S.; Roscher, F.; Schroder, M.; Sieber, G.; Simonis, H. J.; Ulrich, R.; Wagner-Kuhr, J.; Wayand, S.; Weber, M.; Weiler, T.; Williamson, S.; Wohrmann, C.; Wolf, R.] Inst Expt Kernphys, Karlsruhe, Germany.
[Anagnostou, G.; Daskalakis, G.; Geralis, T.; Giakoumopoulou, V. A.; Kyriakis, A.; Loukas, D.; Psallidas, A.; Topsis-Giotis, I.] NCSR Demokritos, Inst Nucl & Particle Phys INPP, Aghia Paraskevi, Greece.
[Agapitos, A.; Kesisoglou, S.; Panagiotou, A.; Saoulidou, N.; Tziaferi, E.] Univ Athens, Athens, Greece.
[Evangelou, I.; Flouris, G.; Foudas, C.; Kokkas, R.; Loukas, N.; Manthos, N.; Papadopoulos, I.; Paradas, E.; Strologas, J.] Univ Ioannina, Ioannina, Greece.
[Horvath, D.; Beni, N.; Czellar, S.; Karancsi, J.; Molnar, J.; Szillasi, Z.] Inst Nucl Res ATOMKI, Debrecen, Hungary.
[Karancsi, J.; Bartok, M.; Makovec, A.; Raics, R.; Trocsanyi, Z. L.; Ujvari, B.] Univ Debrecen, Debrecen, Hungary.
[Choudhury, S.; Mal, P.; Mandal, K.; Sahoo, D. K.; Swain, S. K.] Natl Inst Sci Educ & Res, Bhubaneswar, Orissa, India.
[Bansal, S.; Beri, S. B.; Bhatnagar, V.; Chawla, R.; Gupta, R.; Bhawandeep, U.; Kalsi, A. K.; Kaur, A.; Kaur, M.; Kumar, R.; Mehta, A.; Mittal, M.; Singh, J. B.; Walia, G.] Panjab Univ, Chandigarh, India.
[Kumar, Ashok; Bhardwaj, A.; Choudhary, B. C.; Garg, R. B.; Malhotra, S.; Naimuddin, M.; Nishu, N.; Ranjan, K.; Sharma, R.; Sharma, V.] Univ Delhi, Delhi, India.
[Bhattacharya, S.; Chatterjee, K.; Dey, S.; Dutta, S.; Majumdar, N.; Modak, A.; Mondal, K.; Mukhopadhyay, S.; Roy, A.; Roy, D.; Chowdhury, S. Roy; Sarkar, S.; Sharan, M.] Saha Inst Nucl Phys, Kolkata, India.
[Chudasama, R.; Dutta, D.; Jha, V.; Kumar, V.; Mohanty, A. K.; Pant, L. M.; Shukla, R.; Topkar, A.] Bhabha Atom Res Ctr, Mumbai, Maharashtra, India.
[Mittag, G.; Aziz, T.; Banerjee, S.; Bhowmik, S.; Chatterjee, R. M.; Dewanjee, R. K.; Dugad, S.; Ganguly, S.; Ghosh, S.; Guchait, M.; Gurtu, A.; Jain, Sa.; Kole, G.; Kumar, S.; Mahakud, B.; Maity, M.; Majumder, G.; Mazumdar, K.; Mohanty, G. B.; Parida, B.; Sarkar, T.; Sur, N.; Sutar, B.; Wickramage] Tata Inst Fundamental Res, Mumbai, Maharashtra, India.
[Chauhan, S.; Dube, S.; Kapoor, A.; Kothekar, K.; Sharma, S.] IISER, Pune, Maharashtra, India.
[Bakhshiansohi, H.; Behnamian, H.; Etesami, S. M.; Fahim, A.; Khakzad, M.; Najafabadi, M. Mohammadi; Naseri, M.; Mehdiabadi, S. Paktinat; Hosseinabadi, F. Rezaei; Safarzadeh, B.; Zeinali, M.] Inst Res Fundamental Sci IPM, Tehran, Iran.
[Felcini, M.; Grunewald, M.] Univ Coll Dublin, Dublin, Ireland.
[Abbrescia, M.; Calabria, C.; Caputo, C.; Colaleo, A.; Creanza, D.; Cristella, L.; De Filippis, N.; De Palma, M.; Fiore, L.; Iaselli, G.; Maggi, G.; Maggi, M.; Miniello, G.; My, S.; Nuzzo, S.; Pompili, A.; Pugliese, G.; Radogna, R.; Ranieri, A.; Selvaggi, G.; Silvestris, L.; Venditti, R.] Ist Nazl Fis Nucl, Sez Bari, Bari, Italy.
[Abbrescia, M.; Calabria, C.; Caputo, C.; Cristella, L.; De Palma, M.; Miniello, G.; Nuzzo, S.; Pompili, A.; Radogna, R.; Selvaggi, G.; Venditti, R.] Univ Bari, Bari, Italy.
[Creanza, D.; De Filippis, N.; Iaselli, G.; Maggi, G.; My, S.; Pugliese, G.] Politecn Bari, Bari, Italy.
[Abbiendi, G.; Bonacorsi, D.; Braibant-Giacomelli, S.; Brigliadori, L.; Campanini, R.; Capiluppi, R.; Castro, A.; Cavallo, F. R.; Chhibra, S. S.; Codispoti, G.; Cuffiani, M.; Dallavalle, G. M.; Fabbri, F.; Fanfani, A.; Fasanella, D.; Giacomelli, R.; Grandi, C.; Guiducci, L.; Marcellini, S.; Masetti, G.; Montanari, A.; Navarria, F. L.; Perrotta, A.; Rossi, A. M.; Rovelli, T.; Siroli, G. P.; Tosi, N.] Ist Nazl Fis Nucl, Sez Bologna, Bologna, Italy.
[Bonacorsi, D.; Braibant-Giacomelli, S.; Brigliadori, L.; Campanini, R.; Capiluppi, R.; Castro, A.; Chhibra, S. S.; Codispoti, G.; Cuffiani, M.; Fanfani, A.; Fasanella, D.; Guiducci, L.; Navarria, F. L.; Rossi, A. M.; Rovelli, T.; Siroli, G. P.; Tosi, N.] Univ Bologna, Bologna, Italy.
[Chiorboli, M.; Costa, S.; Di Mattia, A.; Giordano, F.; Potenza, R.; Tricomi, A.; Tuve, C.] Ist Nazl Fis Nucl, Sez Catania, Catania, Italy.
[Cappello, G.; Chiorboli, M.; Costa, S.; Giordano, F.; Potenza, R.; Tricomi, A.; Tuve, C.] Univ Catania, Catania, Italy.
[Barbagli, G.; Ciulli, V.; Civinini, C.; D'Alessandro, R.; Focardi, E.; Gori, V.; Lenzi, R.; Meschini, M.; Paoletti, S.; Sguazzoni, G.; Viliani, L.] Ist Nazl Fis Nucl, Sez Firenze, Florence, Italy.
[Ciulli, V.; D'Alessandro, R.; Focardi, E.; Gori, V.; Lenzi, R.; Viliani, L.] Univ Firenze, Florence, Italy.
[Fabbri, F.; Benussi, L.; Bianco, S.; Piccolo, D.; Primavera, F.] Ist Nazl Fis Nucl, Lab Nazl Frascati, Frascati, Italy.
[Calvelli, V.; Ferro, F.; Lo Vetere, M.; Monge, M. R.; Robutti, E.; Tosi, S.] Ist Nazl Fis Nucl, Sez Genova, Genoa, Italy.
[Calvelli, V.; Lo Vetere, M.; Monge, M. R.; Tosi, S.] Univ Genoa, Genoa, Italy.
[Dinardo, M. E.; Fiorendi, S.; Gennai, S.; Gerosa, R.; Ghezzi, A.; Govoni, R.; Malvezzi, S.; Manzoni, R. A.; Marzocchi, B.; Menasce, D.; Moroni, L.; Paganoni, M.; Pedrini, D.; Ragazzi, S.; Redaelli, N.; de Fatis, T. Tabarelli] Ist Nazl Fis Nucl, Sez Milano Bicocca, Milan, Italy.
[Dinardo, M. E.; Fiorendi, S.; Gerosa, R.; Ghezzi, A.; Govoni, R.; Manzoni, R. A.; Marzocchi, B.; Paganoni, M.; Ragazzi, S.; de Fatis, T. Tabarelli] Univ Milano Bicocca, Milan, Italy.
[Buontempo, S.; Cavallo, N.; Di Guida, S.; Esposito, M.; Fabozzi, F.; Lorio, A. O. M.; Lanza, G.; Lista, L.; Meola, S.; Merola, M.; Paolucci, R.; Sciacca, C.] Ist Nazl Fis Nucl, Sez Napoli, Naples, Italy.
[Esposito, M.; Lorio, A. O. M.; Sciacca, C.] Univ Naples Federico II, Naples, Italy.
[Cavallo, N.; Fabozzi, F.] Univ Basilicata, Potenza, Italy.
[Di Guida, S.; Meola, S.] Univ G Marconi, Rome, Italy.
[Azzi, R.; Bacchetta, N.; Benato, L.; Bisello, D.; Boletti, A.; Carlin, R.; Checchia, R.; Dall'Osso, M.; Dorigo, T.; Dosselli, U.; Fanzago, F.; Gasparini, F.; Gasparini, U.; Gonella, F.; Gozzelino, A.; Lacaprara, S.; Margoni, M.; Meneguzzo, A. T.; Michelotto, M.; Pazzini, J.; Pozzobon, N.; Ronchese, R.; Simonetto, F.; Torassa, E.; Tosi, M.; Zotto, R.; Zucchetta, A.; Zumerle, G.] Ist Nazl Fis Nucl, Sez Padova, Padua, Italy.
[Benato, L.; Bisello, D.; Boletti, A.; Carlin, R.; Dall'Osso, M.; Gasparini, F.; Gasparini, U.; Margoni, M.; Meneguzzo, A. T.; Pazzini, J.; Pozzobon, N.; Ronchese, R.; Simonetto, F.; Tosi, M.; Zotto, R.; Zucchetta, A.; Zumerle, G.] Univ Padua, Padua, Italy.
Univ Trento, Trento, Italy.
[Braghieri, A.; Magnani, A.; Montagna, R.; Ratti, S. P.; Re, V.; Riccardi, C.; Salvini, R.; Vai, I.; Vitulo, P.] Ist Nazl Fis Nucl, Sez Pavia, Pavia, Italy.
[Magnani, A.; Montagna, R.; Ratti, S. P.; Riccardi, C.; Vai, I.; Vitulo, P.] Univ Pavia, Pavia, Italy.
[Solestizi, L. Alunni; Bilei, G. M.; Ciangottini, D.; Fano, L.; Lariccia, R.; Mantovani, G.; Menichelli, M.; Saha, A.; Santocchia, A.] Ist Nazl Fis Nucl, Sez Perugia, Perugia, Italy.
[Solestizi, L. Alunni; Ciangottini, D.; Fano, L.; Lariccia, R.; Mantovani, G.; Santocchia, A.] Univ Perugia, Perugia, Italy.
[Androsov, K.; Azzurri, R.; Bagliesi, G.; Bernardini, J.; Boccali, T.; Castaldi, R.; Ciocci, M. A.; Dell'Orso, R.; Donato, S.; Foa, L.; Giassi, A.; Grippo, M. T.; Ligabue, F.; Lomtadze, T.; Martini, L.; Messineo, A.; Palla, F.; Rizzi, A.; Savoy-Navarro, A.; Serban, A. T.; Spagnolo, R.; Tenchini, R.; Tonelli, G.; Venturi, A.; Verdini, P. G.] Ist Nazl Fis Nucl, Sez Pisa, Pisa, Italy.
[Martini, L.; Messineo, A.; Rizzi, A.; Tonelli, G.] Univ Pisa, Pisa, Italy.
[Donato, S.; Foa, L.; Ligabue, F.] Scuola Normale Super Pisa, Pisa, Italy.
[Barone, L.; Cavallari, F.; D'imperio, G.; Del Re, D.; Diemoz, M.; Gelli, S.; Jorda, C.; Longo, E.; Margaroli, F.; Meridiani, R.; Organtini, G.; Paramatti, R.; Preiato, F.; Rahatlou, S.; Rovelli, C.; Santanastasio, F.; Traczyk, P.] Ist Nazl Fis Nucl, Sez Roma, Rome, Italy.
[Barone, L.; D'imperio, G.; Del Re, D.; Gelli, S.; Longo, E.; Margaroli, F.; Organtini, G.; Preiato, F.; Rahatlou, S.; Santanastasio, F.; Traczyk, P.] Univ Rome, Rome, Italy.
[Amapane, N.; Arcidiacono, R.; Argiro, S.; Arneodo, M.; Bellan, R.; Biino, C.; Cartiglia, N.; Costa, M.; Covarelli, R.; Degano, A.; Demaria, N.; Finco, L.; Kiani, B.; Mariotti, C.; Maselli, S.; Migliore, E.; Monaco, V.; Monteil, E.; Obertino, M. M.; Pacher, L.; Pastrone, N.; Pelliccioni, M.; Angioni, G. L. Pinna; Ravera, F.; Romero, A.; Ruspa, M.; Sacchi, R.; Solano, A.; Staiano, A.] Ist Nazl Fis Nucl, Sez Torino, Turin, Italy.
[Amapane, N.; Argiro, S.; Bellan, R.; Costa, M.; Covarelli, R.; Degano, A.; Finco, L.; Kiani, B.; Migliore, E.; Monaco, V.; Monteil, E.; Obertino, M. M.; Pacher, L.; Angioni, G. L. Pinna; Ravera, F.; Romero, A.; Sacchi, R.; Solano, A.] Univ Torino, Turin, Italy.
[Arcidiacono, R.; Arneodo, M.; Ruspa, M.] Univ Piemonte Orientale, Novara, Italy.
[Belforte, S.; Candelise, V.; Casarsa, M.; Cossutti, F.; Della Ricca, G.; Gobbo, B.; La Licata, C.; Marone, M.; Schizzi, A.; Zanetti, A.] Ist Nazl Fis Nucl, Sez Trieste, Trieste, Italy.
[Candelise, V.; Della Ricca, G.; La Licata, C.; Marone, M.; Schizzi, A.] Univ Trieste, Trieste, Italy.
[Kropivnitskaya, A.; Nam, S. K.] Kangwon Natl Univ, Chunchon, South Korea.
[Kim, D. H.; Kim, G. N.; Kim, M. S.; Kong, D. J.; Lee, S.; Oh, Y. D.; Sakharov, A.; Son, D. C.; Kamon, T.] Kyungpook Natl Univ, Daegu, South Korea.
[Cifuentes, J. A. Brochero; Kim, H.; Kim, T. J.] Chonbuk Natl Univ, Jeonju, South Korea.
[Song, S.] Chonnam Natl Univ, Inst Univ & Elementary Particles, Kwangju, South Korea.
[Lee, S.; Kim, H.; Cho, S.; Choi, S.; Go, Y.; Gyun, D.; Hong, B.; Kim, Y.; Lee, B.; Lee, K.; Lee, K. S.; Lim, J.; Park, S. K.; Roh, Y.] Korea Univ, Seoul, South Korea.
[Yoo, H. D.] Seoul Natl Univ, Seoul, South Korea.
[Kim, H.; Choi, M.; Kim, J. H.; Lee, J. S. H.; Park, I. C.; Ryu, G.; Ryu, M. S.] Univ Seoul, Seoul, South Korea.
[Choi, Y.; Goh, J.; Kim, D.; Kwon, E.; Lee, J.; Yu, I.] Sungkyunkwan Univ, Suwon, South Korea.
[Dudenas, V.; Juodagalvis, A.; Vaitkus, J.] Vilnius Univ, Vilnius, Lithuania.
[Ahmed, I.; Ibrahim, Z. A.; Komaragiri, J. R.; Ali, M. A. B. Md; Idris, F. Mohamad; Abdullah, W. A. T. Wan; Yusli, M. N.; Zolkapli, Z.] Univ Malaya, Natl Ctr Particle Phys, Kuala Lumpur, Malaysia.
[Casimiro Linares, E.; Castilla-Valdez, H.; De La Cruz-Burelo, E.; Heredia-De La Cruz, I.; Hernandez-Almada, A.; Lopez-Fernandez, R.; Mejia Guisao, J.; Sanchez-Hernandez, A.] IPN, Ctr Invest Estudios Avanzados, Mexico City, DF, Mexico.
[Carrillo Moreno, S.; Vazquez Valencia, F.] Univ Iberoamer, Mexico City, DF, Mexico.
[Pedraza, I.; Salazar Ibarguen, H. A.; Uribe Estrada, C.] Benemerita Univ Autonoma Puebla, Puebla, Mexico.
[Morelos Pineda, A.] Univ Autonoma San Luis Potosi, San Luis Potosi, Mexico.
[Krofcheck, D.] Univ Auckland, Auckland, New Zealand.
[Butler, P. H.] Univ Canterbury, Christchurch, New Zealand.
[Ahmad, M.; Ahmad, A.; Hassan, Q.; Hoorani, H. R.; Khan, W. A.; Khurshid, T.; Shoaib, M.; Waqas, M.] Quaid I Azam Univ, Natl Ctr Phys, Islamabad, Pakistan.
[Bialkowska, H.; Bluj, M.; Boimska, B.; Frueboes, T.; Gorski, M.; Kazana, M.; Nawrocki, K.; Romanowska-Rybinska, K.; Szleper, M.; Zalewski, R.] Natl Ctr Nucl Res, Otwock, Poland.
[Brona, G.; Bunkowski, K.; Byszuk, A.; Doroba, K.; Kalinowski, A.; Konecki, M.; Krolikowski, J.; Misiura, M.; Olszewski, M.; Walczak, M.] Univ Warsaw, Inst Expt Phys, Fac Phys, Warsaw, Poland.
[Bargassa, R.; Beirao Da Cruz E Silva, C.; Di Francesco, A.; Faccioli, R.; Ferreira Parracho, P. G.; Gallinaro, M.; Hollar, J.; Leonardo, N.; Lloret Iglesias, L.; Nguyen, F.; Rodrigues Antunes, J.; Seixas, J.; Toldaiev, O.; Vadruccio, D.; Varela, J.; Vischia, R.] Lab Instrumentacao & Fis Expt Particulas, Lisbon, Portugal.
[Finger, M.; Finger, M., Jr.; Tsamalaidze, Z.; Afanasiev, S.; Bunin, R.; Gavrilenko, M.; Golutvin, I.; Gorbunov, I.; Kamenev, A.; Karjavin, V.; Laney, A.; Malakhov, A.; Matveev, V.; Moisenz, R.; Palichik, V.; Perelygin, V.; Shmatov, S.; Shulha, S.; Skatchkov, N.; Smirnov, V.; Zarubin, A.] Joint Inst Nucl Res, Dubna, Russia.
[Golovtsov, V.; Ivanov, Y.; Kim, V.; Kuznetsova, E.; Levchenko, R.; Murzin, V.; Oreshkin, V.; Smirnov, I.; Sulimov, V.; Uvarov, L.; Vavilov, S.; Vorobyev, A.] Petersburg Nucl Phys Inst, St Petersburg, Russia.
[Andreev, Yu.; Dermenev, A.; Gninenko, S.; Golubev, N.; Karneyeu, A.; Kirsanov, M.; Krasnikov, N.; Pashenkov, A.; Tlisov, D.; Toropin, A.] Inst Nucl Res, Moscow, Russia.
[Epshteyn, V.; Gavrilov, V.; Lychkovskaya, N.; Popov, V.; Pozdnyakov, I.; Safronov, G.; Spiridonov, A.; Vlasov, E.; Zhokin, A.; Starodumov, A.; Nikitenko, A.] Inst Theoret & Expt Phys, Moscow, Russia.
[Matveev, V.; Chadeeva, M.; Chistov, R.; Danilov, M.; Rusinov, V.; Tarkovskii, E.; Azarkin, M.; Dremin, I.; Leonidov, A.] Natl Res Nucl Univ, Moscow Engn Phys Inst MEPhI, Moscow, Russia.
[Andreev, V.; Azarkin, M.; Dremin, I.; Kirakosyan, M.; Leonidov, A.; Mesyats, G.; Rusakov, S. V.] PN Lebedev Phys Inst, Moscow, Russia.
[Popov, A.; Zhukov, V.; Katkov, I.; Baskakov, A.; Belyaev, A.; Boos, E.; Demiyanov, A.; Ershov, A.; Gribushin, A.; Kodolova, O.; Korotkikh, V.; Lokhtin, I.; Miagkov, I.; Obraztsov, S.; Petrushanko, S.; Savrin, V.; Snigirev, A.; Vardanyan, I.] Lomonosov Moscow State Unav, Skobeltsyn Inst Nucl Phys, Moscow, Russia.
[Azhgirey, I.; Bayshev, I.; Bitioukov, S.; Kachanov, V.; Kalinin, A.; Konstantinov, D.; Krychkine, V.; Petrov, V.; Ryutin, R.; Sobol, A.; Tourtchanovitch, L.; Troshin, S.; Tyurin, N.; Uzunian, A.; Volkov, A.] State Res Ctr Russian Federat, Inst High Energy Phys, Protvino, Russia.
[Adzic, R.; Cirkovic, R.; Devetak, D.; Milosevic, J.; Rekovic, V.; Milenovic, R.] Univ Belgrade, Fac Phys, Belgrade, Serbia.
[Adzic, R.; Cirkovic, R.; Devetak, D.; Milosevic, J.; Rekovic, V.; Milenovic, R.] Vinca Inst Nucl Sci, Belgrade, Serbia.
[Alcaraz Maestre, J.; Calvo, E.; Cerrada, M.; Chamizo Llatas, M.; Colino, N.; De La Cruz, B.; Delgado Peris, A.; Escalante Del Valle, A.; Fernandez Bedoya, C.; Fernandez Ramos, J. P.; Flix, J.; Fouz, M. C.; Garcia-Abia, R.; Gonzalez Lopez, O.; Goy Lopez, S.; Hernandez, J. M.; Josa, M. I.; Navarro De Martino, E.; Perez-Calero Yzquierdo, A.; Puerta Pelayo, J.; Quintario Olmeda, A.; Redondo, I.; Romero, L.; Santaolalla, J.; Soares, M. S.] Ctr Invest Energet Medioambientales & Tecnol CIEM, Madrid, Spain.
[Albajar, C.; de Troconiz, J. F.; Missiroli, M.; Moran, D.] Univ Autonoma Madrid, Madrid, Spain.
[Cuevas, J.; Fernandez Menendez, J.; Folgueras, S.; Gonzalez Caballero, I.; Palencia Cortezon, E.; Vizan Garcia, J. M.] Univ Oviedo, Oviedo, Spain.
[Cabrillo, I. J.; Calderon, A.; Castineiras De Saa, J. R.; Curras, E.; De Castro Manzano, R.; Fernandez, M.; Garcia-Ferrero, J.; Gomez, G.; Lopez Virto, A.; Marco, J.; Marco, R.; Martinez Rivero, C.; Matorras, F.; Piedra Gomez, J.; Rodrigo, T.; Rodriguez-Marrero, A. Y.; Ruiz-Jimeno, A.; Scodellaro, L.; Trevisani, N.; Vila, I.; Vilar Cortabitarte, R.] Univ Cantabria, CSIC, Inst Fis Cantabria IFCA, Santander, Spain.
[Rabady, D.; Merlin, J. A.; Pantaleo, F.; Hartmann, F.; Kornmayer, A.; Szillasi, Z.; Mohanty, A. K.; Silvestris, L.; Battilana, C.; Tosi, N.; Viliani, L.; Primavera, F.; Manzoni, R. A.; Di Guida, S.; Meola, S.; Paolucci, R.; Azzi, R.; Dall'Osso, M.; Pazzini, J.; Zucchetta, A.; Ciangottini, D.; Azzurri, R.; Donato, S.; Abbaneo, D.; Auffray, E.; Auzinger, G.; Bachtis, M.; Baillon, R.; Ball, A. H.; Barney, D.; Benaglia, A.; Bendavid, J.; Benhabib, L.; Berruti, G. M.; Bloch, R.; Bocci, A.; Bonato, A.; Botta, C.; Breuker, H.; Camporesi, T.; Castello, R.; Cerminara, G.; D'Alfonso, M.; d'Enterria, D.; Dabrowski, A.; Daponte, V.; David, A.; De Gruttola, M.; De Guio, F.; De Roeck, A.; De Visscher, S.; Di Marco, E.; Dobson, M.; Dordevic, M.; Dorney, B.; du Pree, T.; Duggan, D.; Dunser, M.; Dupont, N.; Elliott-Peisert, A.; Franzoni, G.; Fulcher, J.; Funk, W.; Gigi, D.; Gill, K.; Giordano, D.; Girone, M.; Glege, F.; Guida, R.; Gundacker, S.; Guthoff, M.; Hammer, J.; Harris, R.; Hegeman, J.; Innocente, V.; Janot, R.; Kirschenmann, H.; Kortelainen, M. J.; Kousouris, K.; Krajczar, K.; Lecoq, R.; Lourenco, C.; Lucchini, M. T.; Magini, N.; Malgeri, L.; Mannelli, M.; Martelli, A.; Masetti, L.; Meijers, F.; Mersi, S.; Meschi, E.; Moortgat, F.; Morovic, S.; Mulders, M.; Nemallapudi, M. V.; Neugebauer, H.; Orfanelli, S.; Orsini, L.; Pape, L.; Perez, E.; Peruzzi, M.; Petrilli, A.; Petrucciani, G.; Pfeiffer, A.; Pierini, M.; Piparo, D.; Racz, A.; Reis, T.; Rolandi, G.; Rovere, M.; Ruan, M.; Sakulin, H.; Schafer, C.; Schwick, C.; Seidel, M.; Sharma, A.; Silva, R.; Simon, M.; Sphicas, R.; Steggemann, J.; Stieger, B.; Stoye, M.; Takahashi, Y.; Treille, D.; Triossi, A.; Tsirou, A.; Veres, G. I.; Wardle, N.; Wohri, H. K.; Zagozdzinska, A.; Zeuner, W. D.; Ulmer, K. A.] CERN, European Org Nucl Res, Geneva, Switzerland.
[Bertl, W.; Deiters, K.; Erdmann, W.; Horisberger, R.; Ingram, Q.; Kaestli, H. C.; Kotlinski, D.; Langenegger, U.; Rohe, T.] Paul Scherrer Inst, Villigen, Switzerland.
[Bachmair, F.; Bani, L.; Bianchini, L.; Casal, B.; Dissertori, G.; Dittmar, M.; Donega, M.; Eller, R.; Grab, C.; Heidegger, C.; Hits, D.; Hoss, J.; Kasieczka, G.; Lecomte, R.; Lustermann, W.; Mangano, B.; Marionneau, M.; del Arbol, R. Martinez Ruiz; Masciovecchio, M.; Meinhard, M. T.; Meister, D.; Micheli, F.; Musella, R.; Nessi-Tedaldi, F.; Pandolfi, F.; Pata, J.; Pauss, F.; Perrozzi, L.; Quittnat, M.; Rossini, M.; Schonenberger, M.; Starodumov, A.; Takahashi, M.; Tavolaro, V. R.; Theofilatos, K.; Wallny, R.] ETH, Inst Particle Phys, Zurich, Switzerland.
[Aarrestad, T. K.; Amsler, C.; Caminada, L.; Canelli, M. F.; Chiochia, V.; De Cosa, A.; Galloni, C.; Hinzmann, A.; Hreus, T.; Kilminster, B.; Lange, C.; Ngadiuba, J.; Pinna, D.; Rauco, G.; Robmann, R.; Salerno, D.; Yang, Y.] Univ Zurich, Zurich, Switzerland.
[Cardaci, M.; Chen, K. H.; Doan, T. H.; Jain, Sh.; Khurana, R.; Konyushikhin, M.; Kuo, C. M.; Lin, W.; Lu, Y. J.; Pozdnyakov, A.; Yu, S. S.] Natl Cent Univ, Chungli, Taiwan.
[Kumar, Arun; Chang, R.; Chang, Y. H.; Chang, Y. W.; Chao, Y.; Chen, K. F.; Chen, P. H.; Dietz, C.; Fiori, F.; Grundler, U.; Hou, W-S.; Hsiung, Y.; Liu, Y. F.; Lu, R-S.; Moya, M. Minano; Petrakou, E.; Tsai, J. F.; Tzeng, Y. M.] Natl Taiwan Univ, Taipei, Taiwan.
[Asavapibhop, B.; Kovitanggoon, K.; Singh, G.; Srimanobhas, N.; Suwonjandee, N.] Chulalongkorn Univ, Dept Phys, Fac Sci, Bangkok, Thailand.
[Adiguzel, A.; Cerci, S.; Damarseckin, S.; Demiroglu, Z. S.; Dozen, C.; Dumanoglu, I.; Girgis, S.; Gokbulut, G.; Guler, Y.; Gurpinar, E.; Hos, I.; Kanga, E. E.; Topaksu, A. Kayis; Onengut, G.; Ozdemir, K.; Polatoz, A.; Tali, B.; Topakli, H.; Zorbilmez, C.] Cukurova Univ, Adana, Turkey.
[Bilin, B.; Bilmis, S.; Isildak, B.; Karapinar, G.; Yalvac, M.; Zeyrek, M.] Middle East Tech Univ, Dept Phys, Ankara, Turkey.
[Gulmez, E.; Kaya, M.; Kaya, O.; Yetkin, E. A.; Yetkin, T.] Bogazici Univ, Istanbul, Turkey.
[Cakir, A.; Cankocak, K.; Sen, S.; Vardarh, F. I.] Istanbul Tech Univ, Istanbul, Turkey.
[Grynyov, B.] Natl Acad Sci Ukraine, Inst Scintillat Mat, Kharkov, Ukraine.
[Levchuk, L.; Sorokin, R.] Kharkov Inst Phys & Technol, Natl Sci Ctr, Kharkov, Ukraine.
[Aggleton, R.; Ball, F.; Beck, L.; Brooke, J. J.; Clement, E.; Cussans, D.; Flacher, H.; Goldstein, J.; Grimes, M.; Heath, G. P.; Heath, H. F.; Jacob, J.; Kreczko, L.; Lucas, C.; Meng, Z.; Newbold, D. M.; Paramesvaran, S.; Poll, A.; Sakuma, T.; El Nasr-Storey, S. Seif; Senkin, S.; Smith, D.; Smith, V. J.] Univ Bristol, Bristol, Avon, England.
[Newbold, D. M.; Belyaev, A.; Brew, C.; Brown, R. M.; Calligaris, L.; Cieri, D.; Cockerill, D. J. A.; Coughlan, J. A.; Harder, K.; Harper, S.; Olaiya, E.; Petyt, D.; Shepherd-Themistocleous, C. H.; Thea, A.; Tomalin, I. R.; Williams, T.; Worm, S. D.; Lucas, R.] Rutherford Appleton Lab, Didcot, Oxon, England.
[Baber, M.; Bainbridge, R.; Buchmuller, O.; Bundock, A.; Burton, D.; Casasso, S.; Citron, M.; Colling, D.; Corpe, L.; Dauncey, R.; Davies, G.; De Wit, A.; Della Negra, M.; Dunne, R.; Elwood, A.; Futyan, D.; Hall, G.; Iles, G.; Lane, R.; Lucas, R.; Lyons, L.; Magnan, A-M.; Malik, S.; Nash, J.; Nikitenko, A.; Pela, J.; Pesaresi, M.; Raymond, D. M.; Richards, A.; Rose, A.; Seez, C.; Tapper, A.; Uchida, K.; Acosta, M. Vazquez; Virdee, T.; Zenz, S. C.] Imperial Coll, London, England.
[Cole, J. E.; Hobson, P. R.; Khan, A.; Kyberd, R.; Leslie, D.; Reid, I. D.; Symonds, R.; Teodorescu, L.; Turner, M.] Brunel Univ, Uxbridge, Middx, England.
[Borzou, A.; Call, K.; Dittmann, J.; Hatakeyama, K.; Liu, H.; Pastika, N.] Baylor Univ, Waco, TX 76798 USA.
[Charaf, O.; Cooper, S. I.; Henderson, C.; Rumerio, R.] Univ Alabama, Tuscaloosa, AL USA.
[Arcaro, D.; Avetisyan, A.; Bose, T.; Gastler, D.; Rankin, D.; Richardson, C.; Rohlf, J.; Sulak, L.; Zou, D.] Boston Univ, Boston, MA 02215 USA.
[Alimena, J.; Benelli, G.; Berry, E.; Cutts, D.; Ferapontov, A.; Garabedian, A.; Hakala, J.; Heintz, U.; Jesus, O.; Laird, E.; Landsberg, G.; Mao, Z.; Narain, M.; Piperov, S.; Sagir, S.; Syarif, R.] Brown Univ, Providence, RI 02912 USA.
[Breedon, R.; Breto, G.; Sanchez, M. Calderon De La Barca; Chauhan, S.; Chertok, M.; Conway, J.; Conway, R.; Cox, P. T.; Erbacher, R.; Funk, G.; Gardner, M.; Ko, W.; Lander, R.; Mclean, C.; Mulhearn, M.; Pellett, D.; Pilot, J.; Ricci-Tam, F.; Shalhout, S.; Smith, J.; Squires, M.; Stolp, D.; Tripathi, M.; Wilbur, S.; Yohay, R.] Univ Calif Davis, Davis, CA 95616 USA.
[Weber, M.; Cousins, R.; Everaerts, R.; Florent, A.; Hauser, J.; Ignatenko, M.; Saltzberg, D.; Takasugi, E.; Valuev, V.] Univ Calif Los Angeles, Los Angeles, CA USA.
[Burt, K.; Clare, R.; Ellison, J.; Gary, J. W.; Hanson, G.; Heilman, J.; Paneva, M. Ivova; Jandir, R.; Kennedy, E.; Lacroix, F.; Long, O. R.; Malberti, M.; Negrete, M. Olmedo; Shrinivas, A.; Wei, H.; Wimpenny, S.; Yates, B. R.] Univ Calif Riverside, Riverside, CA 92521 USA.
[Branson, J. G.; Cerati, G. B.; Cittolin, S.; D'Agnolo, R. T.; Derdzinski, M.; Holzner, A.; Kelley, R.; Klein, D.; Letts, J.; Macneill, I.; Olivito, D.; Padhi, S.; Pieri, M.; Sani, M.; Sharma, V.; Simon, S.; Tadel, M.; Vartak, A.; Wasserbaech, S.; Welke, C.; Wurthwein, F.; Yagil, A.; Della Porta, G. Zevi] Univ Calif San Diego, La Jolla, CA 92093 USA.
[Bradmiller-Feld, J.; Campagnari, C.; Dishaw, A.; Dutta, V.; Flowers, K.; Sevilla, M. Franco; Geffert, R.; George, C.; Golf, F.; Gouskos, L.; Gran, J.; Incandela, J.; Mccoll, N.; Mullin, S. D.; Richman, J.; Stuart, D.; Suarez, I.; West, C.; Yoo, J.] Univ Calif Santa Barbara, Santa Barbara, CA 93106 USA.
[Anderson, D.; Apresyan, A.; Bornheim, A.; Bunn, J.; Chen, Y.; Duarte, J.; Mott, A.; Newman, H. B.; Pena, C.; Spiropulu, M.; Vlimant, J. R.; Xie, S.; Zhu, R. Y.] CALTECH, Pasadena, CA 91125 USA.
[Andrews, M. B.; Azzolini, V.; Calamba, A.; Carlson, B.; Ferguson, T.; Paulini, M.; Russ, J.; Sun, M.; Vogel, H.; Vorobiev, I.] Carnegie Mellon Univ, Pittsburgh, PA 15213 USA.
[Cumalat, J. P.; Ford, W. T.; Gaz, A.; Jensen, F.; Johnson, A.; Krohn, M.; Mulholland, T.; Nauenberg, U.; Stenson, K.; Wagner, S. R.] Univ Colorado, Boulder, CO 80309 USA.
[Alexander, J.; Chatterjee, A.; Chaves, J.; Chu, J.; Dittmer, S.; Eggert, N.; Mirman, N.; Kaufman, G. Nicolas; Patterson, J. R.; Rinkevicius, A.; Ryd, A.; Skinnari, L.; Soffi, L.; Sun, W.; Tan, S. M.; Teo, W. D.; Thom, J.; Thompson, J.; Tucker, J.; Weng, Y.; Wittich, R.] Cornell Univ, Ithaca, NY USA.
[Abdullin, S.; Albrow, M.; Apollinari, G.; Banerjee, S.; Bauerdick, L. A. T.; Beretvas, A.; Berryhill, J.; Bhat, P. C.; Bolla, G.; Burkett, K.; Butler, J. N.; Cheung, H. W. K.; Chlebana, F.; Cihangir, S.; Elvira, V. D.; Fisk, I.; Freeman, J.; Gottschalk, E.; Gray, L.; Green, D.; Grunendahl, S.; Gutsche, O.; Hanlon, J.; Hare, D.; Harris, R. M.; Hasegawa, S.; Hirschauer, J.; Hu, Z.; Jayatilaka, B.; Jindariani, S.; Johnson, M.; Joshi, U.; Klima, B.; Kreis, B.; Lammel, S.; Lewis, J.; Linacre, J.; Lincoln, D.; Lipton, R.; Liu, T.; De Sa, R. Lopes; Lykken, J.; Maeshima, K.; Marraffino, J. M.; Maruyama, S.; Mason, D.; McBride, R.; Merkel, R.; Mrenna, S.; Nahn, S.; Newman-Holmes, C.; O'Dell, V.; Pedro, K.; Prokofyev, O.; Rakness, G.; Sexton-Kennedy, E.; Soha, A.; Spalding, W. J.; Spiegel, L.; Stoynev, S.; Strobbe, N.; Taylor, L.; Tkaczyk, S.; Tran, N. V.; Uplegger, L.; Vaandering, E. W.; Vernieri, C.; Verzocchi, M.; Vidal, R.; Wang, M.; Weber, H. A.; Whitbeck, A.] Fermilab Natl Accelerator Lab, POB 500, Batavia, IL 60510 USA.
[Acosta, D.; Avery, R.; Bortignon, R.; Bourilkov, D.; Brinkerhoff, A.; Carnes, A.; Carver, M.; Curry, D.; Das, S.; Field, R. D.; Furic, I. K.; Konigsberg, J.; Korytov, A.; Kotov, K.; Ma, R.; Matchev, K.; Mei, H.; Milenovic, R.; Mitselmakher, G.; Rank, D.; Rossin, R.; Shchutska, L.; Snowball, M.; Sperka, D.; Terentyev, N.; Thomas, L.; Wang, J.; Wang, S.; Yelton, J.] Univ Florida, Gainesville, FL USA.
[Hewamanage, S.; Linn, S.; Markowitz, R.; Martinez, G.; Rodriguez, J. L.] Florida Int Univ, Miami, FL 33199 USA.
[Ackert, A.; Adams, J. R.; Adams, T.; Askew, A.; Bein, S.; Bochenek, J.; Diamond, B.; Haas, J.; Hagopian, S.; Hagopian, V.; Johnson, K. F.; Khatiwada, A.; Prosper, H.; Weinberg, M.] Florida State Univ, Tallahassee, FL 32306 USA.
[Baarmand, M. M.; Bhopatkar, V.; Colafranceschi, S.; Hohlmann, M.; Kalakhety, H.; Noonan, D.; Roy, T.; Yumiceva, F.] Florida Inst Technol, Melbourne, FL 32901 USA.
[Adams, M. R.; Apanasevich, L.; Berry, D.; Betts, R. R.; Bucinskaite, I.; Cavanaugh, R.; Evdokimov, O.; Gauthier, L.; Gerber, C. E.; Hofman, D. J.; Kurt, R.; O'Brien, C.; Gonzalez, I. D. Sandoval; Turner, R.; Varelas, N.; Wu, Z.; Zakaria, M.; Zhang, J.] Univ Illinois, Chicago, IL USA.
[Bilki, B.; Clarida, W.; Dilsiz, K.; Durgut, S.; Gandrajula, R. P.; Haytmyradov, M.; Khristenko, V.; Merlo, J. -R; Mermerkaya, H.; Mestvirishvili, A.; Moeller, A.; Nachtman, J.; Ogul, H.; Onel, Y.; Ozok, F.; Penzo, A.; Snyder, C.; Tiras, E.; Wetzel, J.; Yi, K.] Univ Iowa, Iowa City, IA USA.
[Anderson, I.; Barnett, B. A.; Blumenfeld, B.; Cocoros, A.; Eminizer, N.; Fehling, D.; Feng, L.; Gritsan, A. V.; Maksimovic, R.; Osherson, M.; Roskes, J.; Sarica, U.; Swartz, M.; Xiao, M.; Xin, Y.; You, C.] Johns Hopkins Univ, Baltimore, MD USA.
[Baringer, R.; Bean, A.; Bruner, C.; Kenny, R. P., III; Majumder, D.; Malek, M.; Mcbrayer, W.; Murray, M.; Sanders, S.; Stringer, R.; Wang, Q.] Univ Kansas, Lawrence, KS 66045 USA.
[Ivanov, A.; Kaadze, K.; Khalil, S.; Makouski, M.; Maravin, Y.; Mohammadi, A.; Saini, L. K.; Skhirtladze, N.; Toda, S.] Kansas State Univ, Manhattan, KS 66506 USA.
[Lange, D.; Rebassoo, F.; Wright, D.] Lawrence Livermore Natl Lab, Livermore, CA USA.
[Anelli, C.; Baden, A.; Baron, o.; Belloni, A.; Calvert, B.; Eno, S. C.; Ferraioli, C.; Gomez, J. A.; Hadley, N. J.; Jabeen, S.; Kellogg, R. G.; Kolberg, T.; Kunkle, J.; Lu, Y.; Mignerey, A. C.; Shin, Y. H.; Skuja, A.; Tonjes, M. B.; Tonwar, S. C.] Univ Maryland, College Pk, MD 20742 USA.
[Apyan, A.; Barbieri, R.; Baty, A.; Bi, R.; Bierwagen, K.; Brandt, S.; Busza, W.; Cali, I. A.; Demiragli, Z.; Di Matteo, L.; Ceballos, G. Gomez; Goncharov, M.; Gulhan, D.; Iiyama, Y.; Innocenti, G. M.; Klute, M.; Kovalskyi, D.; Lai, Y. S.; Lee, Y-J.; Levin, A.; Luckey, P. D.; Marini, A. C.; Mcginn, C.; Mironov, C.; Narayanan, S.; Niu, X.; Paus, C.; Roland, C.; Roland, G.; Salfeld-Nebgen, J.; Stephans, G. S. F.; Sumorok, K.; Tatar, K.; Varma, M.; Velicanu, D.; Veverka, J.; Wang, J.; Wang, T. W.; Wyslouch, B.; Yang, M.; Zhukova, V.] MIT, Cambridge, MA 02139 USA.
[Benvenuti, A. C.; Dahmes, B.; Evans, A.; Finkel, A.; Gude, A.; Hansen, R.; Kalafut, S.; Kao, S. C.; Klapoetke, K.; Kubota, Y.; Lesko, Z.; Mans, J.; Nourbakhsh, S.; Ruckstuhl, N.; Rusack, R.; Tambe, N.; Turkewitz, J.] Univ Minnesota, Minneapolis, MN USA.
[Acosta, J. G.; Oliveros, S.] Univ Mississippi, Oxford, MS USA.
[Cerci, S.; Avdeeva, E.; Bartek, R.; Bloom, K.; Bose, S.; Claes, D. R.; Dominguez, A.; Fangmeier, C.; Suarez, R. Gonzalez; Kamalieddin, R.; Knowlton, D.; Kravchenko, I.; Meier, F.; Monroy, J.; Ratnikov, F.; Siado, J. E.; Snow, G. R.] Univ Nebraska, Lincoln, NE USA.
[Alyari, M.; Dolen, J.; George, J.; Godshalk, A.; Harrington, C.; Iashvili, I.; Kaisen, J.; Kharchilava, A.; Kumar, A.; Rappoccio, S.; Roozbahani, B.] SUNY Buffalo, Buffalo, NY USA.
[Alverson, G.; Barberis, E.; Baumgartel, D.; Chasco, M.; Hortiangtham, A.; Massironi, A.; Morse, D. M.; Nash, D.; Orimoto, T.; De Lima, R. Teixeira; Trocino, D.; Wang, R. -J.; Wood, D.; Zhang, J.] Northeastern Univ, Boston, MA 02115 USA.
[Bhattacharya, S.; Hahn, K. A.; Kubik, A.; Low, J. F.; Mucia, N.; Odell, N.; Pollack, B.; Schmitt, M.; Sung, K.; Trovato, M.; Velasco, M.] Northwestern Univ, Evanston, IL USA.
[Dev, N.; Hildreth, M.; Jessop, C.; Karmgard, D. J.; Kellams, N.; Lannon, K.; Marinelli, N.; Meng, F.; Mueller, C.; Musienko, Y.; Planer, M.; Reinsvold, A.; Ruchti, R.; Smith, G.; Taroni, S.; Valls, N.; Wayne, M.; Wolf, M.; Woodard, A.] Univ Notre Dame, Notre Dame, IN 46556 USA.
[Antonelli, L.; Brinson, J.; Bylsma, B.; Durkin, L. S.; Flowers, S.; Hart, A.; Hill, C.; Hughes, R.; Ji, W.; Ling, T. Y.; Liu, B.; Luo, W.; Puigh, D.; Rodenburg, M.; Winer, B. L.; Wulsin, H. W.] Ohio State Univ, Columbus, OH 43210 USA.
[Driga, O.; Elmer, R.; Hardenbrook, J.; Hebda, R.; Koay, S. A.; Lujan, R.; Marlow, D.; Medvedeva, T.; Mooney, M.; Olsen, J.; Palmer, C.; Piroue, R.; Stickland, D.; Tully, C.; Zuranski, A.] Princeton Univ, Princeton, NJ 08544 USA.
[Malik, S.] Univ Puerto Rico, Mayaguez, PR USA.
[Savoy-Navarro, A.; Barker, A.; Barnes, V. E.; Benedetti, D.; Bortoletto, D.; Gutay, L.; Jha, M. K.; Jones, M.; Jung, A. W.; Jung, K.; Kumar, A.; Miller, D. H.; Neumeister, N.; Radburn-Smith, B. C.; Shi, X.; Shipsey, I.; Silvers, D.; Sun, J.; Svyatkovskiy, A.; Wang, F.; Xie, W.; Xu, L.] Purdue Univ, W Lafayette, IN 47907 USA.
[Parashar, N.; Stupak, J.] Purdue Univ Calumet, Hammond, LA USA.
[Adair, A.; Akgun, B.; Chen, Z.; Ecklund, K. M.; Geurts, F. J. M.; Guilbaud, M.; Li, W.; Michlin, B.; Northup, M.; Padley, B. P.; Redjimi, R.; Roberts, J.; Rorie, J.; Tu, Z.; Zabel, J.] Rice Univ, Houston, TX USA.
[Betchart, B.; Bodek, A.; de Barbaro, R.; Demina, R.; Eshaq, Y.; Ferbel, T.; Galanti, M.; Garcia-Bellido, A.; Han, J.; Hindrichs, O.; Khukhunaishvili, A.; Lo, K. H.; Tan, R.; Verzetti, M.] Univ Rochester, Rochester, NY 14627 USA.
[Chou, J. P.; Contreras-Campana, E.; Ferencek, D.; Gershtein, Y.; Halkiadakis, E.; Heindl, M.; Hidas, D.; Hughes, E.; Kaplan, S.; Elayavalli, R. Kunnawalkam; Lath, A.; Nash, K.; Saka, H.; Salur, S.; Schnetzer, S.; Sheffield, D.; Somalwar, S.; Stone, R.; Thomas, S.; Thomassen, R.; Walker, M.] Rutgers State Univ, Piscataway, NJ USA.
[Forthomme, L.; Riley, G.; Rose, K.; Spanier, S.; Thapa, K.] Univ Tennessee, Knoxville, TN USA.
[Bouhali, O.; Hernandez, A. Castaneda; Celik, A.; Dalchenko, M.; De Mattia, M.; Delgado, A.; Dildick, S.; Eusebi, R.; Gilmore, J.; Huang, T.; Kamon, T.; Krutelyov, V.; Mueller, R.; Osipenkov, I.; Pakhotin, Y.; Patel, R.; Perloff, A.; Rose, A.; Safonov, A.; Tatarinov, A.; Ulmer, K. A.] Texas A&M Univ, College Stn, TX USA.
[Appelt, E.; Delannoy, A. G.; Greene, S.; Gurrola, A.; Janjam, R.; Johns, W.; Maguire, C.; Mao, Y.; Melo, A.; Ni, H.; Sheldon, R.; Tuo, S.; Velkovska, J.; Xu, Q.] Vanderbilt Univ, 221 Kirkland Hall, Nashville, TN 37235 USA.
[Arenton, M. W.; Cox, B.; Francis, B.; Goodell, J.; Hirosky, R.; Ledovskoy, A.; Li, H.; Lin, C.; Neu, C.; Sinthuprasith, T.; Sun, X.; Wang, Y.; Wolfe, E.; Wood, J.; Xia, F.] Univ Virginia, Charlottesville, VA USA.
[Clarke, C.; Harr, R.; Karchin, P. E.; Don, C. Kottachchi Kankanamge; Lamichhane, R.; Sturdy, J.] Wayne State Univ, Detroit, MI USA.
[Belknap, D. A.; Carlsmith, D.; Cepeda, M.; Dasu, S.; Dodd, L.; Duric, S.; Gomber, B.; Grothe, M.; Herndon, M.; Herve, A.; Klabbers, R.; Lanaro, A.; Levine, A.; Long, K.; Loveless, R.; Mohapatra, A.; Ojalvo, I.; Perry, T.; Pierro, G. A.; Polese, G.; Ruggles, T.; Sarangi, T.; Savin, A.; Sharma, A.; Smith, N.; Smith, W. H.; Taylor, D.; Verwilligen, R.; Woods, N.] Univ Wisconsin, Madison, WI USA.
[Fabjan, C.; Fruhwirth, R.; Jeitler, M.; Krammer, M.; Schieck, J.; Wulz, C. -E.] Vienna Univ Technol, Vienna, Austria.
[Chinellato, J.; Manganote, E. J. Tonelli] Univ Estadual Campinas, Campinas, Brazil.
[Moon, C. S.] CNRS, IN2P3, Paris, France.
[Abdelalim, A. A.; Mahrous, A.] Helwan Univ, Cairo, Egypt.
[Abdelalim, A. A.] Zewail City Sci & Technol, Zewail, Egypt.
[Radi, A.] British Univ Egypt, Cairo, Egypt.
[Radi, A.] Ain Shams Univ, Cairo, Egypt.
[Agram, J. -L.; Conte, E.; Fontaine, J. -C.] Univ Haute Alsace, Mulhouse, France.
[Hempel, M.; Karacheban, O.; Lohmann, W.] Brandenburg Tech Univ Cottbus, Cottbus, Germany.
[Vesztergombi, G.; Veres, G. I.] Eotvos Lorand Univ, Budapest, Hungary.
[Bartok, M.] Wigner Res Ctr Phys, Budapest, Hungary.
[Choudhury, S.] Indian Inst Sci Educ & Res, Bhopal, India.
[Chatterjee, R. M.; Maity, M.; Sarkar, T.] Visva Bharati Univ, Santini Ketan, W Bengal, India.
[Gurtu, A.] King Abdulaziz Univ, Jeddah, Saudi Arabia.
[Wickramage] Univ Ruhuna, Matara, Sri Lanka.
[Etesami, S. M.] Isfahan Univ Technol, Esfahan, Iran.
[Fahim, A.] Univ Tehran, Dept Engn Sci, Tehran, Iran.
[Safarzadeh, B.] Islamic Azad Univ, Sci & Res Branch, Plasma Phys Res Ctr, Tehran, Iran.
[Androsov, K.; Ciocci, M. A.; Grippo, M. T.] Univ Siena, Siena, Italy.
[Ali, M. A. B. Md] Int Islamic Univ Malaysia, Kuala Lumpur, Malaysia.
[Idris, F. Mohamad] Agensi Nuklear Malaysia, MOSTI, Kajang, Malaysia.
[Heredia-De La Cruz, I.] Consejo Nacl Ciencia & Technol, Mexico City, DF, Mexico.
[Byszuk, A.; Zagozdzinska, A.] Warsaw Univ Technol, Inst Elect Syst, Warsaw, Poland.
[Kim, V.] St Petersburg State Polytech Univ, St Petersburg, Russia.
[Rolandi, G.] Scuola Normale, Pisa, Italy.
[Rolandi, G.] Sezione Ist Nazl Fis Nucl, Pisa, Italy.
[Amsler, C.] Albert Einstein Ctr Fundamental Phys, Bern, Switzerland.
[Tali, B.] Adiyaman Univ, Adiyaman, Turkey.
[Kanga, E. E.] Mersin Univ, Mersin, Turkey.
[Onengut, G.] Cag Univ, Mersin, Turkey.
[Ozdemir, K.] Piri Reis Univ, Istanbul, Turkey.
[Topakli, H.] Gaziosmanpasa Univ, Tokat, Turkey.
[Isildak, B.] Ozyegin Univ, Istanbul, Turkey.
[Karapinar, G.] Izmir Inst Technol, Izmir, Turkey.
[Kaya, M.] Marmara Univ, Istanbul, Turkey.
[Kaya, O.] Kafkas Univ, Kars, Turkey.
[Yetkin, E. A.] Istanbul Bilgi Univ, Istanbul, Turkey.
[Yetkin, T.] Yildiz Tech Univ, Istanbul, Turkey.
[Sen, S.] Hacettepe Univ, Ankara, Turkey.
[Belyaev, A.] Univ Southampton, Sch Phys & Astron, Southampton, Hants, England.
[Acosta, M. Vazquez] Inst Astrofis Canarias, San Cristobal la Laguna, Spain.
[Wasserbaech, S.] Utah Valley Univ, Orem, UT USA.
[Colafranceschi, S.] Univ Roma, Fac Ingn, Rome, Italy.
[Bilki, B.] Argonne Natl Lab, 9700 S Cass Ave, Argonne, IL 60439 USA.
[Mermerkaya, H.] Erzincan Univ, Erzincan, Turkey.
[Ozok, F.] Mimar Sinan Univ, Istanbul, Turkey.
[Bouhali, O.; Hernandez, A. Castaneda] Texas A&M Univ Qatar, Doha, Qatar.
[Akchurin, N.; Cowden, C.; Damgov, J.; Dragoiu, C.; Dudero, P. R.; Faulkner, J.; Kunori, S.; Lamichhane, K.; Lee, S. W.; Libeiro, T.; Undleeb, S.; Volobouev, I.] Texas Tech Univ, Lubbock, TX 79409 USA.
RP Khachatryan, V (reprint author), Yerevan Phys Inst, Yerevan, Armenia.
RI Della Ricca, Giuseppe/B-6826-2013; Manganote, Edmilson/K-8251-2013;
Konecki, Marcin/G-4164-2015; Puljak, Ivica/D-8917-2017; TUVE',
Cristina/P-3933-2015; Goh, Junghwan/Q-3720-2016; Lokhtin,
Igor/D-7004-2012
OI Della Ricca, Giuseppe/0000-0003-2831-6982; Konecki,
Marcin/0000-0001-9482-4841; TUVE', Cristina/0000-0003-0739-3153; Goh,
Junghwan/0000-0002-1129-2083;
FU BMWFW (Austria); FWF (Austria); F.R.S. - FNRS (Belgium); CNPq (Brazil);
CAPES (Brazil); FAPERJ (Brazil); FAPESP (Brazil); MES (Bulgaria); CERN;
CAS (China); MOST (China); NSFC (China); COLCIENCIAS (Colombia); MSES
(Croatia); CSF (Croatia); RPF (Cyprus); MoER (Estonia); ERC IUT
(Estonia); ERDF (Estonia); Academy of Finland (Finland); MEC (Finland);
HIP (Finland); CEA (France); CNRS/IN2P3 (France); BMBF (Germany); DFG
(Germany); HGF (Germany); GSRT (Greece); OTKA (Hungary); NIH (Hungary);
DAE (India); DST (India); IPM (Iran); SFI (Ireland); INFN (Italy); MSIP
(Republic of Korea); NRF (Republic of Korea); LAS (Lithuania); MOE
(Malaysia); UM (Malaysia); CINVESTAV (Mexico); CONACYT (Mexico); SEP
(Mexico); UASLP-FAI (Mexico); MBIE (New Zealand); PAEC (Pakistan); MSHE
(Poland); NSC (Poland); FCT (Portugal); JINR (Dubna); MON (Russia);
RosAtom (Russia); RAS (Russia); RFBR (Russia); MESTD (Serbia); SEIDI
(Spain); CPAN (Spain); Swiss Funding Agencies (Switzerland); MST
(Taipei); ThEPCenter (Thailand); IPST (Thailand); STAR (Thailand); NSTDA
(Thailand); TUBITAK (Turkey); TAEK (Turkey); NASU (Ukraine); SFFR
(Ukraine); STFC (United Kingdom); DOE (USA); NSF (USA); Marie-Curie
programme; European Research Council; EPLANET (European Union); Leventis
Foundation; Alfred P. Sloan Foundation; Alexander von Humboldt
Foundation; Belgian Federal Science Policy Office; Fonds pour la
Formation a la Recherche dans l'Industrie et dans l'Agriculture
(FRIA-Belgium); Agentschap voor Innovatie door Wetenschap en Technologie
(IWT-Belgium); Ministry of Education, Youth and Sports (MEYS) of the
Czech Republic; Council of Science and Industrial Research, India;
HOMING PLUS programme of the Foundation for Polish Science; European
Union, Regional Development Fund; OPUS programme of the National Science
Center (Poland); Compagnia di San Paolo (Torino); MIUR (Italy)
[20108T4XTM]; Thalis programme - EU-ESF; Aristeia programme - EU-ESF;
Greek NSRF; National Priorities Research Program by Qatar National
Research Fund; Rachadapisek Sompot Fund for Postdoctoral Fellowship,
Chulalongkorn University (Thailand); Chulalongkorn Academic into Its 2nd
Century Project Advancement Project (Thailand); Welch Foundation
[C-1845]
FX We congratulate our colleagues in the CERN accelerator departments for
the excellent performance of the LHC and thank the technical and
administrative staffs at CERN and at other CMS institutes for their
contributions to the success of the CMS effort. In addition, we
gratefully acknowledge the computing centres and personnel of the
Worldwide LHC Computing Grid for delivering so effectively the computing
infrastructure essential to our analyses. Finally, we acknowledge the
enduring support for the construction and operation of the LHC and the
CMS detector provided by the following funding agencies: BMWFW and FWF
(Austria); F.R.S. - FNRS and FWO (Belgium); CNPq, CAPES, FAPERJ, and
FAPESP (Brazil); MES (Bulgaria); CERN; CAS, MOST, and NSFC (China);
COLCIENCIAS (Colombia); MSES and CSF (Croatia); RPF (Cyprus); MoER, ERC
IUT and ERDF (Estonia); Academy of Finland, MEC, and HIP (Finland); CEA
and CNRS/IN2P3 (France); BMBF, DFG, and HGF (Germany); GSRT (Greece);
OTKA and NIH (Hungary); DAE and DST (India); IPM (Iran); SFI (Ireland);
INFN (Italy); MSIP and NRF (Republic of Korea); LAS (Lithuania); MOE and
UM (Malaysia); CINVESTAV, CONACYT, SEP, and UASLP-FAI (Mexico); MBIE
(New Zealand); PAEC (Pakistan); MSHE and NSC (Poland); FCT (Portugal);
JINR (Dubna); MON, RosAtom, RAS and RFBR (Russia); MESTD (Serbia); SEIDI
and CPAN (Spain); Swiss Funding Agencies (Switzerland); MST (Taipei);
ThEPCenter, IPST, STAR and NSTDA (Thailand); TUBITAK and TAEK (Turkey);
NASU and SFFR (Ukraine); STFC (United Kingdom); DOE and NSF (USA).;
Individuals have received support from the Marie-Curie programme and the
European Research Council and EPLANET (European Union); the Leventis
Foundation; the Alfred P. Sloan Foundation; the Alexander von Humboldt
Foundation; the Belgian Federal Science Policy Office; the Fonds pour la
Formation a la Recherche dans l'Industrie et dans l'Agriculture
(FRIA-Belgium); the Agentschap voor Innovatie door Wetenschap en
Technologie (IWT-Belgium); the Ministry of Education, Youth and Sports
(MEYS) of the Czech Republic; the Council of Science and Industrial
Research, India; the HOMING PLUS programme of the Foundation for Polish
Science, cofinanced from European Union, Regional Development Fund; the
OPUS programme of the National Science Center (Poland); the Compagnia di
San Paolo (Torino); MIUR project 20108T4XTM (Italy); the Thalis and
Aristeia programmes cofinanced by EU-ESF and the Greek NSRF; the
National Priorities Research Program by Qatar National Research Fund;
the Rachadapisek Sompot Fund for Postdoctoral Fellowship, Chulalongkorn
University (Thailand); the Chulalongkorn Academic into Its 2nd Century
Project Advancement Project (Thailand); and the Welch Foundation,
contract C-1845.
NR 25
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PU ELSEVIER SCIENCE BV
PI AMSTERDAM
PA PO BOX 211, 1000 AE AMSTERDAM, NETHERLANDS
SN 0370-2693
EI 1873-2445
J9 PHYS LETT B
JI Phys. Lett. B
PD OCT 10
PY 2016
VL 761
BP 31
EP 52
DI 10.1016/j.physletb.2016.07.065
PG 22
WC Astronomy & Astrophysics; Physics, Nuclear; Physics, Particles & Fields
SC Astronomy & Astrophysics; Physics
GA DX6CI
UT WOS:000384469900006
ER
PT J
AU Va'vra, J
AF Va'vra, J.
TI More on molecular excitations: Dark matter detection in ice
SO PHYSICS LETTERS B
LA English
DT Article
DE Ice Cube experiment; Dark matter search
ID H2O ICE
AB In this paper we investigate di-atomic molecules embedded in ice crystals under strain. In this environment coherent vibrations of many OH-bonds may be generated by one WIMP collision. The detection of such multiple-photon signals may provide a signature of a 100 GeV/c(2) WIMP. To do a proper lab test of "WIMP-induced" multi-photon emission is very difficult. We suggest that Ice Cube make a search for multi-photon events, and investigate whether the rate of such events exhibits yearly modulation. Published by Elsevier B.V.
C1 [Va'vra, J.] Stanford Univ, SLAC, Stanford, CA 94309 USA.
RP Va'vra, J (reprint author), Stanford Univ, SLAC, Stanford, CA 94309 USA.
EM jjv@slac.stanford.edu
NR 9
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U1 0
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PU ELSEVIER SCIENCE BV
PI AMSTERDAM
PA PO BOX 211, 1000 AE AMSTERDAM, NETHERLANDS
SN 0370-2693
EI 1873-2445
J9 PHYS LETT B
JI Phys. Lett. B
PD OCT 10
PY 2016
VL 761
BP 58
EP 61
DI 10.1016/j.physletb.2016.08.014
PG 4
WC Astronomy & Astrophysics; Physics, Nuclear; Physics, Particles & Fields
SC Astronomy & Astrophysics; Physics
GA DX6CI
UT WOS:000384469900008
ER
PT J
AU Nomura, Y
Salzetta, N
AF Nomura, Yasunori
Salzetta, Nico
TI Why firewalls need not exist
SO PHYSICS LETTERS B
LA English
DT Article
ID GENERALIZED 2ND LAW; BLACK-HOLE; INFLATIONARY UNIVERSE; ENTROPY;
THERMODYNAMICS; RADIATION; DYNAMICS
AB The firewall paradox for black holes is often viewed as indicating a conflict between unitarity and the equivalence principle. We elucidate how the paradox manifests as a limitation of semiclassical theory, rather than presents a conflict between fundamental principles. Two principal features of the fundamental and semiclassical theories address two versions of the paradox: the entanglement and typicality arguments. First, the physical Hilbert space describing excitations on a fixed black hole background in the semiclassical theory is exponentially smaller than the number of physical states in the fundamental theory of quantum gravity. Second, in addition to the Hilbert space for physical excitations, the semiclassical theory possesses an unphysically large Fock space built by creation and annihilation operators on the fixed black hole background. Understanding these features not only eliminates the necessity of firewalls but also leads to a new picture of Hawking emission contrasting pair creation at the horizon. (C) 2016 The Authors. Published by Elsevier B.V.
C1 [Nomura, Yasunori; Salzetta, Nico] Univ Calif Berkeley, Dept Phys, Berkeley Ctr Theoret Phys, Berkeley, CA 94720 USA.
[Nomura, Yasunori; Salzetta, Nico] Lawrence Berkeley Natl Lab, Theoret Phys Grp, Berkeley, CA 94720 USA.
RP Salzetta, N (reprint author), Univ Calif Berkeley, Dept Phys, Berkeley Ctr Theoret Phys, Berkeley, CA 94720 USA.; Salzetta, N (reprint author), Lawrence Berkeley Natl Lab, Theoret Phys Grp, Berkeley, CA 94720 USA.
EM nsalzetta@berkeley.edu
OI Nomura, Yasunori/0000-0002-1497-1479
FU Office of Science, Office of High Energy and Nuclear Physics, of the
U.S. Department of Energy [DE-AC02-05CH11231]; National Science
Foundation [PHY-1521446]; MEXT KAKENHI Grant [15H05895]
FX This work was supported in part by the Director, Office of Science,
Office of High Energy and Nuclear Physics, of the U.S. Department of
Energy under Contract DE-AC02-05CH11231, the National Science Foundation
under grant PHY-1521446, and MEXT KAKENHI Grant Number 15H05895.
NR 47
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PI AMSTERDAM
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SN 0370-2693
EI 1873-2445
J9 PHYS LETT B
JI Phys. Lett. B
PD OCT 10
PY 2016
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BP 62
EP 69
DI 10.1016/j.physletb.2016.08.003
PG 8
WC Astronomy & Astrophysics; Physics, Nuclear; Physics, Particles & Fields
SC Astronomy & Astrophysics; Physics
GA DX6CI
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PT J
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TI Measurement of the t(t)over-bar production cross-section using e mu
events with b-tagged jets in pp collisions at root s=13 TeV with the
ATLAS detector
SO PHYSICS LETTERS B
LA English
DT Article
ID PARTON DISTRIBUTIONS; HADRON COLLIDERS; PLUS PLUS; LHC
AB This paper describes a measurement of the inclusive top quark pair production cross-section (sigma(t (t) over bar)) with a data sample of 3.2 fb(-1) of proton-proton collisions at a centre-of-mass energy of root s = 13 TeV, collected in 2015 by the ATLAS detector at the LHC. This measurement uses events with an opposite-charge electron-muon pair in the final state. Jets containing b-quarks are tagged using an algorithm based on track impact parameters and reconstructed secondary vertices. The numbers of events with exactly one and exactly two b-tagged jets are counted and used to determine simultaneously sigma(t (t) over bar) and the efficiency to reconstruct and b-tag a jet from a top quark decay, thereby minimising the associated systematic uncertainties. The cross-section is measured to be:
s(t (t) over bar)= 818 +/- 8 (stat) +/- 27 (syst) +/- 19 (lumi) +/- 12 (beam) pb,
where the four uncertainties arise from data statistics, experimental and theoretical systematic effects, the integrated luminosity and the LHC beam energy, giving a total relative uncertainty of 4.4%. The result is consistent with theoretical QCD calculations at next-to-next-to-leading order. A fiducial measurement corresponding to the experimental acceptance of the leptons is also presented. (C) 2016 The Author(s). Published by Elsevier B.V.
C1 [Acharya, B. S.; Jackson, P.; Lee, L.; Petridis, A.; White, M. J.] Univ Adelaide, Dept Phys, Adelaide, SA, Australia.
[Ahmadov, F.; Bouffard, J.; Ernst, J.; Fischer, A.; Guindon, S.; Huseynov, N.; Jain, V.; Javadov, N.] SUNY Albany, Dept Phys, Albany, NY 12222 USA.
[Anisenkov, A. V.; Baldin, E. M.; Bobrovnikov, V. S.; Buzykaev, A. R.; Czodrowski, P.; Dassoulas, J.; Dehghanian, N.; Gingrich, D. M.; Jabbar, S.; Karamaoun, A.; Kazanin, V. F.; Kharlamov, A. G.; Korol, A. A.; Mann, A; Maslennikov, A. L.; Maximov, D. A.; Moore, R. W.; Peleganchuk, S. V.; Pinfold, J. L.; Rezanova, O. L.; Soukharev, A. M.; Talyshev, A. A.; Tikhonov, Yu. A.] Univ Alberta, Dept Phys, Edmonton, AB, Canada.
[Cakira, O.; Ciftci, A. K.; Yildiz, H. Duran] Ankara Univ, Dept Phys, Ankara, Turkey.
Istanbul Aydin Univ, Istanbul, Turkey.
[Sultansoy, S.] TOBB Univ Econ & Technol, Div Phys, Ankara, Turkey.
[Banerjee, Sw.; Barnovska, Z.; Berger, N.; Delmastro, M.; Di Ciaccio, L.; Elles, S.; Grevtsov, K.; Guillemin, T.; Hryn'ova, T.; Jezequel, S.; Koletsou, I.; Lafaye, R.; Leveque, J.; Mann, A; Mastrandrea, P.; Sauvage, G.; Sauvan, E.; Simard, O.; Smart, B. H.; Todorov, T.; Wingerter-Seez, I.; Yatsenko, E.] CNRS IN2P3, LAPP, Annecy Le Vieux, France.
[Banerjee, Sw.; Barnovska, Z.; Berger, N.; Delmastro, M.; Di Ciaccio, L.; Elles, S.; Grevtsov, K.; Guillemin, T.; Hryn'ova, T.; Jezequel, S.; Koletsou, I.; Lafaye, R.; Leveque, J.; Mastrandrea, P.; Sauvage, G.; Sauvan, E.; Simard, O.; Smart, B. H.; Todorov, T.; Wingerter-Seez, I.; Yatsenko, E.] Univ Savoie Mt Blanc, Annecy Le Vieux, France.
[Bawa, H. S.; Blair, R. E.; Chekanov, S.; Gao, Y. S.; LeCompte, T.; Love, J.; Malon, D.; Metcalfe, J. .; Nguyen, D. H.; Nodulman, L.; Paramonov, A.; Price, L. E.; Proudfoot, J.; Ryu, S.; Stanek, R. W.; van Gemmeren, P.; Wang, R.; Webster, J. S.; Yoshida, R.; Zhang, J.] Argonne Natl Lab, Div High Energy Phys, Argonne, IL 60439 USA.
[Beck, H. P.; Cheu, E.; Johns, K. A.; Jones, S.; Lamp, W.; Lei, X.; Leone, R.; Loch, P.; Nayyar, R.; O'grady, F.; Rutherfoord, J. P.; Shupe, M. A.; Varnes, E. W.] Univ Arizona, Dept Phys, Tucson, AZ 85721 USA.
[Aloisio, A.; Brandt, A.; Bullock, D.; Casado, M. P.; Darmora, S.; De, K.; Farbin, A.; Feremenga, L.; Griffiths, J.; Hadavand, H. K.; Heelan, L.; Kim, H. Y.; Mann, A; Ozturk, N.; Schovancova, J.; Stradling, A. R.; Usai, G.; Vartapetian, A.; White, A.; Yu, J.] Univ Texas Arlington, Dept Phys, POB 19059, Arlington, TX 76019 USA.
[Angelidakis, S.; Castro, N. F.; Chouridou, S.; Fassouliotis, D.; Giokaris, N.; Ioannou, P.; Kourkoumelis, C.; Tsirintanis, N.] Univ Athens, Dept Phys, Athens, Greece.
[Alexopoulos, T.; Benekos, N.; Chelkov, G. A.; Dris, M.; Gazis, E. N.; Karakostas, K.; Karastathis, N.; Karentzos, E.; Leontsinis, S.; Maltezos, S.; Ntekas, K.; Panagiotopoulou, E. St.; Papadopoulou, Th. D.; Tsipolitis, G.; Vlachos, S.] Natl Tech Univ Athens, Dept Phys, Zografos, Greece.
[Andeen, T.; Conventi, F.; Della Pietra, M.; Ilchenko, Y.; Narayan, R.; Onyisi, P. U. E.] Univ Texas Austin, Dept Phys, Austin, TX 78712 USA.
[Abdinov, O.; Corriveau, F.; Khalil-Zada, F.; McPherson, R. A.; Robertson, S. H.; Sobie, R.; Teuscher, R. J.] Azerbaijan Acad Sci, Inst Phys, Baku, Azerbaijan.
[Anjos, N.; Bosman, M.; Casado, M. P.; Casolino, M.; Cavallaro, E.; Cavalli-Sforza, M.; Cortes-Gonzalez, A.; Ducu, O. A.; Farooque, T.; Perez, S. Fernandez; Fischer, C.; Fracchia, S.; Gerbaudo, D.; Parra, G. Gonzalez; Grinstein, S.; Rozas, A. Juste; Korolkov, I.; Lange, J. C.; Paz, I. Lopez; Martinez, M.; Mir, L. M.; Pages, A. Pacheco; Aranda, C. Padilla; Riu, I.; Rizzi, C.; Perez, A. Rodriguez; Sorin, V.; Tripiana, M. F.; Tsiskaridze, S.; Valery, L.] Barcelona Inst Sci & Technol, Inst Fis Altes Energies IFAE, Barcelona, Spain.
[Abulaiti, Y.; Agatonovic-Jovin, T.; Bogavac, D.; Bokan, P.; Campoverde, A.; Dimitrievska, A.; Fedin, O. L.; Krstic, J.; Marjanovic, M.; Popovic, D. S.; Sijacki, Dj.; Simic, Lj.; Vranjes, N.; Milosavljevic, M. Vranjes; Zivkovic, L.] Univ Belgrade, Inst Phys, Belgrade, Serbia.
[Buanes, T.; Dale, O.; Eigen, G.; Geng, C.; Guo, Y.; Kastanas, A.; Li, B.; Liebig, W.; Lipniacka, A.; Maeland, S.; Latour, B. Martin Dit; Smestad, L.; Stugu, B.; Yang, Z.; Zalieckas, J.] Univ Bergen, Dept Phys & Technol, Bergen, Norway.
[Amadio, B. T.; Axen, B.; Barnett, R. M.; Beringer, J.; Bhimji, W.; Brosamer, J.; Calafiura, P.; Cerutti, F.; Ciocio, A.; Clarke, R. N.; Cooke, M.; Duffield, E. M.; Einsweiler, K.; Farrell, S.; Gabrielli, A.; Garcia-Sciveres, M.; Gilchriese, M.; Govender, N.; Haber, C.; Heim, T.; Heinemann, B.; Hinchliffe, I.; Hinman, R. R.; Holmes, T. R.; Jeanty, L.; Leggett, C.; Marshall, Z.; Ohm, C. C.; Griso, S. Pagan; Potamianos, K.; Pranko, A.; Shapiro, M.; Sood, A.; Tibbetts, M. J.; Trottier-McDonald, M.; Tsulaia, V.; Viel, S.; Wang, H.; Yao, W-M.; Yu, D. R.] Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Div Phys, Berkeley, CA 94720 USA.
[Amadio, B. T.; Axen, B.; Barnett, R. M.; Beringer, J.; Bhimji, W.; Brosamer, J.; Calafiura, P.; Cerutti, F.; Ciocio, A.; Clarke, R. N.; Cooke, M.; Duffield, E. M.; Einsweiler, K.; Farrell, S.; Gabrielli, A.; Garcia-Sciveres, M.; Gilchriese, M.; Govender, N.; Haber, C.; Heim, T.; Heinemann, B.; Hinchliffe, I.; Hinman, R. R.; Holmes, T. R.; Jeanty, L.; Leggett, C.; Marshall, Z.; Ohm, C. C.; Griso, S. Pagan; Potamianos, K.; Pranko, A.; Shapiro, M.; Sood, A.; Tibbetts, M. J.; Trottier-McDonald, M.; Tsulaia, V.; Viel, S.; Wang, H.; Yao, W-M.; Yu, D. R.] Univ Calif Berkeley, Berkeley, CA 94720 USA.
[Biedermann, D.; Dietrich, J.; Giorgi, F. M.; Grancagnolo, S.; Greenwood, Z. D.; Herbert, G. H.; Hristova, I.; Kind, O. M.; Kolanoski, H.; Lacker, H.; Lohse, T.; Mergelmeyer, S.; Nikiforov, A.; Rehnisch, L.; Rieck, P.; Sawyer, L.; Schulz, H.; Sperlich, D.; Stamm, S.; zur Nedden, M.] Humboldt Univ, Dept Phys, Berlin, Germany.
[Aloisio, A.; Beck, H. P.; Cervelli, A.; Ereditato, A.; Rozas, A. Juste; Mann, A; Martinez, M.; Meloni, F.; Mullier, G. A.; Rimoldi, M.; Stramaglia, M. E.; Weber, M. S.] Univ Bern, Albert Einstein Ctr Fundamental Phys, Bern, Switzerland.
[Beck, H. P.; Cervelli, A.; Ereditato, A.; Grinstein, S.; Haug, S.; Rozas, A. Juste; Mann, A; Martinez, M.; Meloni, F.; Mullier, G. A.; Rimoldi, M.; Stramaglia, M. E.; Stucci, S. A.; Weber, M. S.] Univ Bern, High Energy Phys Lab, Bern, Switzerland.
[Allport, Rr; Bella, L. Aperio; Baca, M. J.; Bracinik, J.; Broughton, J. H.; Casadei, D.; Charlton, D. G.; Chisholm, A. S.; Daniells, A. C.; Foster, A. G.; Gonella, L.; Hanagaki, K.; Hawkes, C. M.; Head, S. J.; Levy, M.; Mann, A; Mudd, R. D.; Quijada, J. A. Murillo; Newman, P. R.; Nikolopoulos, K.; Owen, R. E.; Slater, M.; Thomas, J. P.; Thompson, Rd.; Watkins, P. M.; Watson, A. T.; Watson, M. F.; Wilson, J. A.] Univ Birmingham, Sch Phys & Astron, Birmingham, W Midlands, England.
[Arik, M.; Istin, S.; Ozcan, V. E.] Bogazici Univ, Dept Phys, Istanbul, Turkey.
[Beddall, A.; Bingul, A.] Gaziantep Univ, Dept Engn Phys, Gaziantep, Turkey.
[Cetin, S. A.] Istanbul Bilgi Univ, Fac Engn & Nat Sci, Istanbul, Turkey.
[Beddall, A. J.] Bahcesehir Univ, Fac Engn & Nat Sci, Istanbul, Turkey.
[Igonkina, O.; Losada, M.; Moreno, D.; Navarro, G.; Sandoval, C.] Univ Antonio Narino, Ctr Invest, Bogota, Colombia.
[Alberghi, G. L.; Bellagamba, L.; Biondi, S.; Boscherini, D.; Bruni, A.; Bruni, G.; Bruschi, M.; D'amen, G.; De Castro, S.; Fabbri, F.; Fabbri, L.; Franchini, M.; Gabrielli, A.; Giacobbe, B.; Giorgi, F. M.; Grafstroem, R.; Mann, A; Massa, I.; Massa, L.; Mengarelli, A.; Negrini, M.; Piccinini, M.; Polini, A.; Rinaldi, L.; Romano, M.; Sbarra, C.; Sbrizzi, A.; Semprini-Cesari, N.; Sidoti, A.; Sioli, M.; Spighi, R.; Tupputi, S. A.; Ucchielli, G.; Valentinetti, S.; Villa, M.; Vittori, C.; Zoccoli, A.] Ist Nazl Fis Nucl, Sez Bologna, Bologna, Italy.
[Alberghi, G. L.; Biondi, S.; D'amen, G.; Fabbri, F.; Fabbri, L.; Franchini, M.; Gabrielli, A.; Grafstroem, R.; Mann, A; Massa, I.; Massa, L.; Mengarelli, A.; Piccinini, M.; Romano, M.; Sbrizzi, A.; Semprini-Cesari, N.; Sidoti, A.; Sioli, M.; Tupputi, S. A.; Ucchielli, G.; Valentinetti, S.; Villa, M.; Vittori, C.; Zoccoli, A.] Univ Bologna, Dipartimento Fis & Astron, Bologna, Italy.
[Arslan, O.; Bechtle, R.; Bernlochner, F. U.; Brock, I.; Bruscino, N.; Cioara, I. A.; Cristinziani, M.; Desch, K.; Dingfelder, J.; Gaycken, G.; Geich-Gimbel, Ch.; Ghneimat, M.; Grefe, C.; Haefner, R.; Hageboeck, S.; Hansen, M. C.; Hohn, D.; Huegging, F.; Janssen, J.; Jenni, P.; Kraus, J. K.; Kroseberg, J.; Krueger, H.; Lantzsch, K.; Lassnig, M.; Lenz, T.; Leyko, A. M.; Liebal, J.; Mann, A; Mijovic, L.; Moles-Valls, R.; Pohl, D.; Ricken, O.; Sarrazin, B.; Schaepe, S.; Schopf, E.; Schultens, M. J.; Seema, P.; Stillings, J. A.; von Toerne, E.; Wagner, P.; Wermes, N.; Wienemann, P.; Wiik-Fuchs, L. A. M.; Winter, B. T.; Wong, K. H. Yau; Yuen, S. P. Y.; Zhang, R.] Univ Bonn, Phys Inst, Bonn, Germany.
[Ahlen, S. P.; Black, K. M.; Butler, J. M.; Dell'Asta, L.; Helary, L.; Khubua, J.; Kruskal, M.; Long, B. A.; Shank, J. T.; Yan, Z.; Youssef, S.] Boston Univ, Dept Phys, 590 Commonwealth Ave, Boston, MA 02215 USA.
[Amelung, C.; Amundsen, G.; Barone, G.; Bensinger, J. R.; Bianchini, L.; Blocker, C.; Coffey, L.; Dhaliwal, S.; Kono, T.; Loew, K. M.; Nagai, R.; Sciolla, G.; Venturini, A.; Zengel, K.] Brandeis Univ, Dept Phys, Waltham, MA 02254 USA.
[Coutinho, Y. Amaral; Caloba, L. P.; Maidantchik, C.; Marroquim, F.; Nepomuceno, A. A.; Seixas, J. M.] Univ Fed Rio de Janeiro, COPPE EE IF, Rio De Janeiro, Brazil.
[Cerqueira, A. S.; de Andrade Filho, L. Manhaes; Peralva, B. S.] Fed Univ Juiz de Fora UFJF, Elect Circuits Dept, Juiz De Fora, Brazil.
[do Vale, M. A. B.] Fed Univ Sao Joao del Rei UFSJ, Sao Joao Del Rei, Brazil.
[Donadelli, M.; Navarro, J. L. La Rosa; Leite, M. A. L.] Univ Sao Paulo, Inst Fis, Sao Paulo, Brazil.
[Adams, D. L.; Chen, H.; Gibbard, B.; Lakovidis, G.; Klimentov, A.; Kravchenko, A.; Lanni, F.; Manghi, F. Lasagni; Lee, C. A.; Leisos, A.; Liu, H.; Lynn, D.; Ma, H.; Mountricha, E.; Damazio, D. Oliveira; Paige, F.; Perepelitsa, D. V.; Redlinger, G.; Takai, H.; Tricoli, A.; Undrus, A.] Brookhaven Natl Lab, Dept Phys, Upton, NY 11973 USA.
Transilvania Univ Brasov, Brasov, Romania.
[Alexa, C.; Caprini, I.; Caprini, M.; Chitan, A.; Ciubancann, M.; Constantinescu, S.; Dita, P.; Dita, S.; Dobre, M.; Mann, A; Martoiu, V. S.; Maurer, J.; Olariu, A.; Pantea, D.; Rotaru, M.; Stoicea, G.; Tudorache, A.; Tudorache, V.] Natl Inst Phys & Nucl Engn, Bucharest, Romania.
[Popeneciu, G. A.] Natl Inst Res & Dev Isotop & Mol Technol, Dept Phys, Cluj Napoca, Romania.
Univ Politehn Bucuresti, Bucharest, Romania.
[Gravila, P. M.] West Univ Timisoara, Timisoara, Romania.
[Sola, J. D. Bossio; Liu, B.; Marceca, G.; Otero y Garzon, G.; Piegaia, R.; Reisin, H.; Sacerdoti, S.] Univ Buenos Aires, Dept Fis, Buenos Aires, DF, Argentina.
[Arratia, M.; Barlow, N.; Batley, J. R.; Brochu, F. M.; Brunt, B. H.; Carter, J. R.; Chapman, J. D.; Cottin, G.; Gillam, T. P. S.; Hill, J. C.; Kaneti, S.; Lester, C. G.; Mueller, T.; Myagkov, A. G.; Nikolaenko, V.; Parker, M. A.; Potter, C. J.; Robinson, D.; Rosten, J. H. N.; Thomson, M.; Ward, C. P.; Yusuff, I.; Zaitsev, A. M.] Univ Cambridge, Cavendish Lab, Cambridge, England.
[Bellerive, A.; Cree, G.; Di Valentino, D.; Gillberg, D.; Koffas, T.; Lacey, J.; Leight, W. A.; Nessi, M.; Nomidis, I.; Oakham, F. G.; Pasztor, G.; Ruiz-Martinez, A.; Vincter, M. G.] Carleton Univ, Dept Phys, Ottawa, ON, Canada.
[Aleksa, M.; Aloisio, A.; Alonso, A.; Gonzalez, B. Alvarez; Amoroso, S.; Anders, G.; Anghinolfi, F.; Arnaez, O.; Avolio, G.; Baak, M. A.; Backes, M.; Backhaus, M.; Barak, L.; Beermann, T. A.; Beltramello, O.; Bianco, M.; Bogaerts, J. A.; Bortfeldt, J.; Boveia, A.; Boyd, J.; Burckhart, H.; Camarda, S.; Campana, S.; Garrido, M. D. M. Capeans; Carli, T.; Carrillo-Montoya, G. D.; Catinaccio, A.; Cattai, A.; Cerv, M.; Chromek-Burckhart, D.; Colombo, T.; Conti, G.; Dell'Acqua, A.; Deviveiros, P. O.; Di Girolamo, A.; Di Girolamo, B.; Di Nardo, R.; Dittus, F.; Dobos, D.; Dudarev, A.; Duehrssen, M.; Eifert, T.; Ellis, N.; Elsing, M.; Faltova, J.; Farthouat, R.; Fassnacht, P.; Feng, E. J.; Francis, D.; Fressard-Batraneanu, S. M.; Froidevaux, D.; Gadatsch, S.; Goossens, L.; Gorini, B.; Gray, H. M.; Gumpert, C.; Hawkings, R. J.; Helsens, C.; Correia, A. M. Henriques; Hervas, L.; Huhtinen, M.; Iengo, P.; Jakobsen, S.; Klioutchnikova, T.; Krasznahorkay, A.; Lapoire, C.; Law, A. T.; Miotto, G. Lehmann; Lenzi, B.; Lichard, P.; Malyukov, S.; Mandelli, B.; Mann, A; Mapelli, L.; Marzin, A.; Berlingen, J. Montejo; Mornacchi, G.; Nairz, A. M.; Nakahama, Y.; Nessi, M.; Nordberg, M.; Oide, H.; Palestini, S.; Pasztor, G.; Pauly, T.; Pernegger, H.; Petersen, B. A.; Pommes, K.; Poppleton, A.; Poulard, G.; Poveda, J.; Astigarraga, M. E. Pozo; Rammensee, M.; Raymond, M.; Rembser, C.; Ritsch, E.; Roe, S.; Ruthmann, N.; Salzburger, A.; Schaefer, D.; Schlenker, S.; Schmieden, K.; Sforza, F.; Sanchez, C. A. Solans; Spigu, G.; Starz, S.; Stelzer, H. J.; Teischinger, F. A.; Ten Kate, H.; Unal, G.; van Woerden, M. C.; Vandelli, W.; Voss, R.; Vuillermet, R.; Wells, P. S.; Wengler, T.; Wenig, S.; Werner, P.; Wilkens, H. G.; Wotschack, J.; Young, C. J. S.; Zwalinski, L.] CERN, Geneva, Switzerland.
[Alison, J.; Anderson, K. J.; Bryant, P.; Toro, R. Camacho; Cheng, Y.; Dandoy, J. R.; Facini, G.; Gardner, R. W.; Kapliy, A.; Kim, Y. K.; Krizka, K.; Li, H. L.; Merritt, F. S.; Miller, D. W.; Okumura, Y.; Oreglia, M. J.; Piacquadio, G.; Pilcher, J. E.; Saxon, J.; Shochet, M. J.; Stark, G. H.; Swiatlowski, M.; Vukotic, I.; Wu, M.] Univ Chicago, Enrico Fermi Inst, 5640 S Ellis Ave, Chicago, IL 60637 USA.
[Blunier, S.; Diaz, M. A.; Ochoa-Ricoux, J. P.] Pontificia Univ Catolica Chile, Dept Fis, Santiago, Chile.
[Brooks, W. K.; Carquin, E.; Pezoa, R.; Prokoshin, F.; Loyola, J. E. Salazar; Araya, S. Tapia; White, R.] Univ Tecn Federico Santa Maria, Dept Fis, Valparaiso, Chile.
[da Costa, J. Barreiro Guimaraes; Cheng, H. J.; Fang, Y.; Jin, S.; Li, Q.; Liang, Z.; Merino, J. Llorente; Mann, A; Mansour, J. D.; Ouyang, Q.; Peng, C.; Ren, H.; Shan, L. Y.; Sun, X.; Xu, D.; Zhu, H.; Zhuang, X.] Chinese Acad Sci, Inst High Energy Phys, Beijing, Peoples R China.
[Gao, J.; Geng, C.; Guo, Y.; Han, L.; Hu, Q.; Jiang, Y.; Liu, J. B.; Liu, M.; Liu, Y. L.; Liu, Y.; Mann, A; Peng, H.; Song, H. Y.; Wang, W.; Zhang, G.; Zhang, R.; Zhao, Z.; Zhu, Y.] Univ Sci & Technol China, Dept Modern Phys, Hefei, Anhui, Peoples R China.
[Chen, S.; Wang, C.; Zhang, H.] Nanjing Univ, Dept Phys, Nanjing, Jiangsu, Peoples R China.
[Du, Y.; Feng, C.; Ma, L. L.; Ma, Y.; Wang, C.; Zaidan, R.; Zhang, X.; Zhao, Y.; Zhu, C. G.] Shandong Univ, Sch Phys, Jinan, Shandong, Peoples R China.
[Bret, M. Cano; Guo, J.; Li, L.; Yang, H.] Shanghai Jiao Tong Univ, Dept Phys & Astron, Shanghai Key Lab Particle Phys & Cosmol, Shanghai, Peoples R China.
[Chen, X.; Zhou, N.] Tsinghua Univ, Dept Phys, Beijing 100084, Peoples R China.
[Boumediene, D.; Busato, E.; Calvet, D.; Calvet, S.; Chomont, A. R.; Donini, J. .; Gris, Ph.; Madar, R.; Mann, A; Pallin, D.; Saez, S. M. Romano; Santoni, C.; Shi, L.; Simon, D.; Vazeille, F.] Clermont Univ, Phys Corpusculaire Lab, Clermont Ferrand, France.
[Boumediene, D.; Busato, E.; Calvet, D.; Calvet, S.; Chomont, A. R.; Donini, J. .; Gris, Ph.; Madar, R.; Pallin, D.; Saez, S. M. Romano; Santoni, C.; Shi, L.; Simon, D.; Vazeille, F.] Univ Blaise Pascal, Clermont Ferrand, France.
[Boumediene, D.; Busato, E.; Calvet, D.; Calvet, S.; Chomont, A. R.; Donini, J. .; Gris, Ph.; Madar, R.; Pallin, D.; Saez, S. M. Romano; Santoni, C.; Shi, L.; Simon, D.; Vazeille, F.] CNRS IN2P3, Clermont Ferrand, France.
[Alkire, S. P.; Angerami, A.; Brooijmans, G.; Carbone, R. M.; Clark, M. R.; Cole, B.; Hu, D.; Hughes, E. W.; Iordanidou, K.; Klein, M. H.; Mohapatra, S.; Ochoa, I.; Parsons, J. A.; Shiyakova, M.; Smith, M. N. K.; Smith, R. W.; Thompson, E. N.; Tuts, P. M.; Wang, T.; Zhou, L.] Columbia Univ, Nevis Lab, Irvington, NY USA.
[Alonso, A.; Besjes, G. J.; Dam, M.; Galster, G.; Hansen, J. B.; Hansen, J. D.; Hansen, P. H.; Loevschall-Jensen, A. E.; Monk, J.; Mortensen, S. S.; Pedersen, L. E.; Petersen, T. C.; Pinge, A.; Smirnova, L. N.; Turchikhin, S.; Wiglesworth, C.; Xella, S.] Univ Copenhagen, Niels Bohr Inst, Copenhagen, Denmark.
[Cairo, V. M.; Camplani, A.; Capua, M.; Crosetti, G.; Del Gaudio, M.; La Rotonda, L.; Mastroberardino, A.; Palazzo, S.; Policicchio, A.; Salvatore, D.; Scarfone, V.; Schioppa, M.; Susinno, G.; Tassi, E.] Univ Calabria, INFN Grp Collegato Cosenza, Lab Nazl Frascati, Arcavacata Di Rende, Italy.
[Cairo, V. M.; Camplani, A.; Capua, M.; Crosetti, G.; Del Gaudio, M.; La Rotonda, L.; Mastroberardino, A.; Palazzo, S.; Policicchio, A.; Salvatore, D.; Scarfone, V.; Schioppa, M.; Susinno, G.; Tassi, E.] Univ Calabria, Dipartimento Fis, Arcavacata Di Rende, Italy.
[Adamczyk, L.; Bold, T.; Dabrowski, W.; Gach, G. P.; Grabowska-Bold, I.; Kisielewska, D.; Koperny, S.; Kowalski, T. Z.; Mindur, B.; Przybycien, M.; Zemla, A.] AGH Univ Sci & Technol, Fac Phys & Appl Comp Sci, Krakow, Poland.
[Palka, M.; Richter-Was, E.] Jagiellonian Univ, Marian Smoluchowski Inst Phys, Krakow, Poland.
[Banas, E.; de Renstrom, P. A. Bruckman; Burka, K.; Chwastowski, J. J.; Derendarz, D.; Godlewski, J.; Gornicki, E.; Hajduk, Z.; Kaczmarska, A.; Knapik, J. .; Korcyl, K.; Kowalewska, A. B.; Malecki, Pa.; Mann, A; Olszewski, A.; Olszowska, J.; Stanecka, E.; Staszewski, R.; Tompkins, L.; Trzebinski, M.; Trzupek, A.; Wolter, M. W.; Wosiek, B. K.; Wozniak, K. W.; Zabinski, B.] Polish Acad Sci, Inst Nucl Phys, Krakow, Poland.
[Cao, T.; Firan, A.; Hetherly, J. W.; Kama, S.; Kehoe, R.; Sekula, S. J.; Stroynowski, R.; Toth, J.; Turvey, A. J.; Varol, T.; Wang, H.; Ye, J.; Zhao, X.; Zhou, L.] So Methodist Univ, Dept Phys, Dallas, TX 75275 USA.
[Izen, J. M.; Leyton, M.; Meirose, B.; Namasivayam, H.; Reeves, K.; Vest, A.] Univ Texas Dallas, Dept Phys, Richardson, TX 75083 USA.
[Aloisio, A.; Alonso, A.; Amorim, A.; Andreazza, A.; Angerami, A.; Annovi, A.; Asbah, N.; Behr, J. K.; Bertsche, C.; Bessner, M.; Bloch, I.; Britzger, D.; Deterre, C.; Dutta, B.; Dyndal, M.; Eckardt, C.; Filipuzzi, M.; Flaschel, N.; Bravo, A. Gascon; Gregor, I. M.; Haleem, M.; Hamnett, P. G.; Hiller, K. H.; Howarth, J.; Huang, Y.; Katzy, J.; Keller, J. S.; Kondrashova, N.; Kuh, T.; Lobodzinska, E.; Lohwasser, K.; Madsen, A.; Mann, A; Medinnis, M.; Moenig, K.; Garcia, R. F. Naranjo; Naumann, T.; O'Rourke, A. A.; Peschke, R.; Peters, K.; Pirumov, H.; Poley, A.; Robinson, J. E. M.; Schaefer, R.; Schmitt, S.; South, D.; Stanescu-Bellu, M.; Stanitzki, M. M.; Styles, N. A.; Tackmann, K.; Trofymov, A.; Wang, J.; Yusuff, I.; Zakharchuk, N.] DESY, Hamburg, Germany.
[Aloisio, A.; Asbah, N.; Behr, J. K.; Bertsche, C.; Bessner, M.; Bloch, I.; Britzger, D.; Deterre, C.; Dutta, B.; Dyndal, M.; Eckardt, C.; Filipuzzi, M.; Flaschel, N.; Bravo, A. Gascon; Gregor, I. M.; Haleem, M.; Hamnett, P. G.; Hiller, K. H.; Howarth, J.; Huang, Y.; Katzy, J.; Keller, J. S.; Kondrashova, N.; Kuh, T.; Lobodzinska, E.; Lohwasser, K.; Madsen, A.; Mann, A; Medinnis, M.; Moenig, K.; Garcia, R. F. Naranjo; Naumann, T.; O'Rourke, A. A.; Peschke, R.; Peters, K.; Pirumov, H.; Poley, A.; Robinson, J. E. M.; Schaefer, R.; Schmitt, S.; South, D.; Stanescu-Bellu, M.; Stanitzki, M. M.; Styles, N. A.; Tackmann, K.; Trofymov, A.; Wang, J.; Yusuff, I.; Zakharchuk, N.] DESY, Zeuthen, Germany.
[Burmeister, I.; Cinca, D.; Dette, K.; Erdmann, J.; Esch, H.; Gonella, G.; Goessling, C.; Grohs, J. P.; Homann, M.; Jentzsch, J.; Klingenberg, R.; Kroeninger, K.; Zhang, R.] Tech Univ Dortmund, Lehrstuhl Expt Phys 4, Dortmund, Germany.
[Anger, R.; Duschinger, D.; Friedrich, F.; Gutschow, C.; Hauswald, L.; Kobel, M.; Mader, W. F.; Mann, A; Novgorodova, O.; Siegert, F.; Socher, F.; Straessner, A.; Vest, A.; Wahrmund, S.] Tech Univ Dresden, Inst Kern & Teilchenphys, Dresden, Germany.
[Arce, A. T. H.; Benjamin, D. P.; Bjergaard, D. M.; Bocci, A.; Cerio, B. C.; Goshaw, A. T.; Kajomovitz, E.; Kotwal, A.; Kruse, M. C.; Li, L.; Li, S.; Liu, M.; Oh, S. H.; Zhou, C.] Duke Univ, Dept Phys, Durham, NC 27706 USA.
[Bristow, T. M.; Clark, P. J.; Dias, F. A.; Edwards, N. C.; Gao, Y.; Walls, F. M. Garay; Glaysher, P. C. F.; Harrington, R. D.; Leonidopoulos, C.; Martin, V. J.; Mills, C.; Pino, S. A. Olivares; Proissl, M.; Washbrook, A.; Wynne, B. M.] Univ Edinburgh, SUPA Sch Phys & Astron, Edinburgh, Midlothian, Scotland.
[Antonelli, M.; Beretta, M.; Bilokon, H.; Chiarella, V.; Curatolo, M.; Esposito, B.; Gatti, C.; Maccarrone, G.; Mancini, G.; Sansoni, A.; Testa, M.; Vilucchi, E.] Ist Nazl Fis Nucl, Lab Nazl Frascati, Frascati, Italy.
[Arnold, H.; Betancourt, C.; Boehler, M.; Bruneliere, R.; Buehrer, F.; Burgard, C. D.; Buescher, D.; Cardillo, F.; Coniavitis, E.; Consorti, V.; Dang, N. P.; Dao, V.; Di Simone, A.; Glatzer, J.; Herten, G.; Hirose, M.; Jakobs, K.; Javurek, T.; Jenni, P.; Kiss, F.; Koeneke, K.; Kopp, A. K.; Kuehn, S.; Landgraf, U.; Luedtke, C.; Mann, A; Nagel, M.; Pagacova, M.; Parzefall, U.; Ronzani, M.; Rosbach, K.; Ruhr, F.; Rurikova, Z.; Sammel, D.; Schillo, C.; Schnoor, U.; Schumacher, M.; Sommer, P.; Sundermann, J. E.; Ta, D.; Temming, K. K.; Tsiskaridze, V.; Weiser, C.; Werner, M.; Zhang, L.; Zimmermann, S.] Albert Ludwigs Univ, Fak Math & Phys, Freiburg, Germany.
[Ancu, L. S.; De Mendizaba, J. Bilbao; Calace, N.; Chatterjee, A.; Clark, A.; Coccaro, A.; Delitzsch, C. M.; della Volpe, D.; Ferrere, D.; Gadomski, S.; Golling, T.; Gonzalez-Sevilla, S.; Gramling, J.; Guescini, F.; Lacobucci, G.; Katre, A.; Khoo, T. J.; Lionti, A. E.; Mann, A; March, L.; Mermod, P.; Miucci, A.; Nackenhorst, O.; Paolozzi, L.; Ristic, B.; Schramm, S.; Sfyrla, A.; Vallecorsa, S.; Wu, X.] Univ Geneva, Sect Phys, Geneva, Switzerland.
[Barberis, D.; Darbo, G.; Favareto, A.; Parodi, A. Ferretto; Gagliardi, G.; Gaudiello, A.; Gemme, C.; Guido, E.; Mann, A; Miglioranzi, S.; Morettini, P.; Osculati, B.; Parodi, F.; Passaggio, S.; Rossi, L. P.; Sannino, M.; Schiavi, C.] Ist Nazl Fis Nucl, Sez Genova, Genoa, Italy.
[Barberis, D.; Favareto, A.; Parodi, A. Ferretto; Gagliardi, G.; Gaudiello, A.; Guido, E.; Miglioranzi, S.; Osculati, B.; Parodi, F.; Sannino, M.; Schiavi, C.] Univ Genoa, Dipartimento Fis, Genoa, Italy.
[Tskhadadze, E. G.] Iv Javakhishvili Tbilisi State Univ, E Andronikashvili Inst Phys, Tbilisi, Rep of Georgia.
[Djobava, T.; Durglishvili, A.; Khubua, J.; Mosidze, M.] Tbilisi State Univ, Inst High Energy Phys, Tbilisi, Rep of Georgia.
[Dueren, M.; Heinz, C.; Kreutzfeldt, K.; Stenzel, H.] Justus Liebig Univ Giessen, Phys Inst 2, Giessen, Germany.
[Aloisio, A.; Bates, R. L.; Boutle, S. K.; Madden, W. D. Breaden; Britton, D.; Buckley, A. G.; Bussey, P.; Buttar, C. M.; Buzatu, A.; Crawley, S. J.; D'Auria, S.; Doyle, A. T.; Ferrando, J.; Gul, U.; Knue, A.; Mann, A; Mullen, P.; O'Shea, V.; Owen, M.; Pollard, C. S.; Qin, G.; Quilty, D.; Ravenscroft, T.; Robson, A.; St Denis, R. D.; Stewart, G. A.; Thompson, A. S.] Univ Glasgow, SUPA Sch Phys & Astron, Glasgow, Lanark, Scotland.
[Agricola, J.; Bindi, M.; Blumenschein, U.; Brandt, G.; De Maria, A.; Drechsler, E.; Graber, L.; Grosse-Knetter, J.; Janus, M.; Kareem, M. J.; Lai, S.; Lemmer, B.; Magradze, E.; Mantoani, M.; Mchedlidze, G.; Llacer, M. Moreno; Musheghyan, H.; Quadt, A.; Rieger, J.; Rosien, N. -A.; Rzehorz, G. F.; Shabalina, E.; Stoke, P.; Veatch, J.; Weingarten, J.; Zinonos, Z.] Georg August Univ, Phys Inst 2, Gottingen, Germany.
[Albrand, S.; Berlendis, S.; Camincher, C.; Collot, J.; Crepe-Renaudin, S.; Delsart, P. A.; Gabaldon, C.; Genest, M. H.; Gradin, P. O. J.; Hostachy, J-Y.; Ledroit-Guillon, F.; Lleres, A.; Lucotte, A.; Malek, F.; Petit, E.; Stark, J.; Trocme, B.; Wu, M.] Univ Grenoble Alpes, Lab Phys Subatom & Cosmol, CNRS IN2P3, Grenoble, France.
[McFarlane, K. W.] Hampton Univ, Dept Phys, Hampton, VA 23668 USA.
[Chan, S. K.; Clark, B. L.; Franklin, M.; Giromini, P.; Huth, J.; Ippolito, V.; Lazovich, T.; Mateos, D. Lopez; Morii, M.; Rogan, C. S.; Skottowe, H. P.; Sun, S.; Tolley, E.; Tong, B.; Tuna, A. N.; Yen, A. L.; Zambito, S.] Harvard Univ, Lab Particle Phys & Cosmol, Cambridge, MA 02138 USA.
[Andrei, V.; Antel, C.; Baas, A. E.; Brandt, O.; Djuvsland, J. I.; Dunford, M.; Geisler, M. P.; Hanke, R.; Jongmanns, J.; Kluge, E. -E.; Lang, V. S.; Meier, K.; Zu Theenhausen, H. Meyer; Villar, D. I. Narrias; Sahinsoy, M.; Scharf, V.; Schultz-Coulon, H. -C.; Stamen, R.; Starovoitov, P.; Suchek, S.; Wessels, M.] Heidelberg Univ, Kirchhoff Inst Phys, Heidelberg, Germany.
[Anders, C. F.; de Lima, D. E. Ferreira; Giulini, M.; Kolb, M.; Lisovyi, M.; Radescu, V.; Schaetzel, S.; Schoening, A.; Sosa, D.] Heidelberg Univ, Phys Inst, Heidelberg, Germany.
[Kretz, M.; Kugel, A.] Heidelberg Univ, ZITI Inst Tech Informat, Mannheim, Germany.
[Nagasaka, Y.] Hiroshima Inst Technol, Fac Appl Informat Sci, Hiroshima, Japan.
[Bortolotto, V.; Chan, Y. L.; Castillo, L. R. Flores; Lu, H.; Salvucci, A.; Tsui, K. M.] Chinese Univ Hong Kong, Dept Phys, Shatin, Hong Kong, Peoples R China.
[Bortolotto, V.; Orlando, N.] Univ Hong Kong, Dept Phys, Hong Kong, Hong Kong, Peoples R China.
[Bortolotto, V.; Prokofiev, K.] Hong Kong Univ Sci & Technol, Dept Phys, Clear Water Bay, Kowloon, Hong Kong, Peoples R China.
[Choi, K.; Dattagupta, A.; Evans, H.; Gagnon, P.; Kopeliansky, R.; Lammers, S.; Martinez, N. Lorenzo; Luehring, F.; Ogren, H.; Penwell, J.; Weinert, B.; Zieminska, D.] Indiana Univ, Dept Phys, Bloomington, IN 47405 USA.
[Guenther, J.; Iwanski, W.; Jansky, R.; Kneringer, E.; Lukas, W.; Milic, A.; Usanova, A.; Vigne, R.] Leopold Franzens Univ, Inst Astro & Teilchenphys, Innsbruck, Austria.
[Abdallah, J.; Argyropoulos, S.; Benitez, J.; Mallik, U.] Univ Iowa, Iowa City, IA USA.
[Chen, C.; Cochran, J.; De Lorenzi, F.; Jiang, H.; Krumnack, N.; Pluth, D.; Prell, S.; Werner, M. D.; Yu, J.] Iowa State Univ, Dept Phys & Astron, Ames, IA USA.
[Ahmadov, F.; Aleksandrov, I. N.; Bednyakov, V. A.; Boyko, I. R.; Budagov, I. A.; Chelkov, G. A.; Cheplakov, A.; Chizhov, M. V.; Dedovich, D. V.; Demichev, A.; Gongadze, A.; Gostkin, M. I.; Huseynov, N.; Javadov, N.; Karpov, S. N.; Karpova, Z. M.; Khramov, E.; Kruchonak, U.; Kukhtin, V.; Ladygin, E.; Lyubushkin, V.; Mann, A; Minashvili, I. A.; Mineev, M.; Peshekhonov, V. D.; Plotnikova, E.; Potrap, I. N.; Pozdnyakov, V.; Rusakovich, N. A.; Sadykov, R.; Sapronov, A.; Shiyakova, M.; Soloshenko, A.; Vinogradov, V. B.; Yeletskikh, I.; Zhemchugov, A.; Zimine, N. I.] JINR Dubna, Joint Inst Nucl Res, Dubna, Russia.
[Amako, K.; Aoki, M.; Arai, Y.; Hanagaki, K.; Ikegami, Y.; Ikeno, M.; Iwasaki, H.; Kanzaki, J.; Kondo, T.; Kono, T.; Makida, Y.; Mann, A; Nagai, R.; Nagano, K.; Nakamura, K.; Nozaki, M.; Odaka, S.; Okuyama, T.; Sasaki, O.; Suzuki, S.; Takubo, Y.; Tanaka, S.; Terada, S.; Tokushuku, K.; Tsuno, S.; Unno, Y.; Yamamoto, A.; Yasu, Y.] KEK, High Energy Accelerator Res Org, Tsukuba, Ibaraki, Japan.
[Hasegawa, M.; Kurashige, H.; Maeda, J.; Ochi, A.; Yakabe, R.; Yuan, L.] Kobe Univ, Grad Sch Sci, Kobe, Hyogo, Japan.
[Ishino, M.; Kunigo, T.; Monden, R.; Sumida, T.; Tashiro, T.] Kyoto Univ, Fac Sci, Kyoto, Japan.
[Takashima, R.] Kyoto Univ, Kyoto, Japan.
[Kawagoe, K.; Oda, S.; Otono, H.; Tojo, J. .] Kyushu Univ, Dept Phys, Fukuoka, Japan.
[Verzini, M. J. Alconada; Alonso, F.; Arduh, F. A.; Dova, M. T.; Monticelli, F.; Wahlberg, H.] Univ Nacl La Plata, Inst Fis La Plata, La Plata, Buenos Aires, Argentina.
[Verzini, M. J. Alconada; Alonso, F.; Arduh, F. A.; Dova, M. T.; Monticelli, F.; Wahlberg, H.] Consejo Nacl Invest Cient & Tecn, La Plata, Buenos Aires, Argentina.
[Barton, A. E.; Beattie, M. D.; Bertram, I. A.; Borissov, G.; Bouhova-Thacker, E. V.; Cheatham, S.; Dearnaley, W. J.; Fox, H.; Grimm, K.; Henderson, R. C. W.; Hughes, G.; Jones, R. W. L.; Kartvelishvili, V.; Long, R. E.; Love, P. A.; Muenstermann, D.; Parker, A. J.; Skinner, M. B.; Smizanska, M.; Walder, J. J.; Wharton, A. M.] Univ Lancaster, Dept Phys, Lancaster, England.
[Aliev, M.; Bachas, K.; Chiodini, G.; Gorini, E.; Longo, L.; Primavera, M.; Reale, M.; Spagnolo, S.; Ventura, A.] Univ Salento, Sez Lecce, Ist Nazl Fis Nucl, Lecce, Italy.
[Aliev, M.; Bachas, K.; Gorini, E.; Longo, L.; Reale, M.; Spagnolo, S.; Ventura, A.] Univ Salento, Dipartimento Matemat & Fis, Lecce, Italy.
[Affolder, A. A.; Anders, J. K.; Burdin, S.; D'Onofrio, M.; Dervan, P.; Gwilliam, C. B.; Hayward, H. S.; Jackson, M.; Jones, T. J.; King, B. T.; Klein, M.; Klein, U.; Kretzschmar, J.; Lehan, A.; Maxfield, S. J.; Mehta, A.; Readioff, N. P.; Vossebeld, J. H.] Univ Liverpool, Oliver Lodge Lab, Liverpool, Merseyside, England.
[Cindro, V.; Deliyergiyev, M.; Filipcic, A.; Gorisek, A.; Kanjir, L.; Kersevan, B. P.; Kramberger, G.; Macek, B.; Mandic, I.; Mikuz, M.; Muskinja, M.; Sfiligoj, T.; Sokhrannyi, G.] Jozef Stefan Inst, Dept Phys, Ljubljana, Slovenia.
[Cindro, V.; Deliyergiyev, M.; Filipcic, A.; Gorisek, A.; Kanjir, L.; Kersevan, B. P.; Kramberger, G.; Macek, B.; Mandic, I.; Mikuz, M.; Muskinja, M.; Sfiligoj, T.; Sokhrannyi, G.] Univ Ljubljana, Ljubljana, Slovenia.
[Armitage, L. J.; Bevan, A. J.; Bona, M.; Cerrito, L.; Hays, J. M.; Hickling, R.; Landon, M. P. J.; Lewis, D.; Lloyd, S. L.; Mann, A; Morris, J. D.; Nooney, T.; Piccaro, E.; Rizvi, E.; Sandbach, R. L.] Queen Mary Univ London, Sch Phys & Astron, London, England.
[Berry, T.; Blanco, J. E.; Boisvert, V.; Brooks, T.; Connelly, I. A.; Cowan, G.; Duguid, L.; Giannelli, M. Faucci; George, S.; Gibson, S. M.; Kempster, J. J.; Vazquez, J. G. Panduro; Pastore, Fr.; Savage, G.; Sowden, B. C.; Spano, F.; Teixeira-Dias, P.; Thomas-Wilsker, J.] Royal Holloway Univ London, Dept Phys, Surrey, England.
[Bell, A. S.; Butterworth, J. M.; Campanelli, M.; Christodoulou, V.; Cooper, B. D.; Davison, P.; Falla, R. J.; Freeborn, D.; Gregersen, K.; Ortiz, N. G. Gutierrez; Hesketh, G. G.; Jansen, E.; Jiggins, S.; Konstantinidis, N.; Korn, A.; Kucuk, H.; Leney, K. J. C.; Martyniuk, A. C.; McClymont, L. I.; Mcfayden, J. A.; Nurse, E.; Richter, S.; Scanlon, T.; Sherwood, P.; Simmons, B.; Wardrope, D. R.; Waugh, B. M.] UCL, Dept Phys & Astron, London, England.
[Greenwood, Z. D.; Grossi, G. C.; Jana, D. K.; Sawyer, L.; Subramaniam, R.] Louisiana Tech Univ, Ruston, LA 71270 USA.
[Beau, T.; Bomben, M.; Calderini, G.; Crescioli, F.; De Cecco, S.; Demilly, A.; Derue, F.; Francavilla, P.; Krasny, M. W.; Lacour, D.; Laforge, B.; Laplace, S.; Lavrijsen, W.; Le Dortz, O.; Lefebvre, G.; Solis, A. Lopez; Luzi, P. M.; Malaescu, B.; Marchiori, G.; Nikolic-Audit, I.; Ocariz, J.; Pandini, C. E.; Pires, S.; Ridel, M.; Roos, L.; Trincaz-Duvoid, S.; Varouchas, D.; Yap, Y. C.] UPMC, Lab Phys Nucl & Hautes Energies, Paris, France.
[Beau, T.; Bomben, M.; Calderini, G.; Crescioli, F.; De Cecco, S.; Demilly, A.; Derue, F.; Francavilla, P.; Krasny, M. W.; Lacour, D.; Laforge, B.; Laplace, S.; Lavrijsen, W.; Le Dortz, O.; Lefebvre, G.; Solis, A. Lopez; Luzi, P. M.; Malaescu, B.; Mann, A; Marchiori, G.; Nikolic-Audit, I.; Ocariz, J.; Pandini, C. E.; Pires, S.; Ridel, M.; Roos, L.; Trincaz-Duvoid, S.; Varouchas, D.; Yap, Y. C.] Univ Paris Diderot, Paris, France.
[Beau, T.; Bomben, M.; Calderini, G.; Crescioli, F.; De Cecco, S.; Demilly, A.; Derue, F.; Francavilla, P.; Krasny, M. W.; Lacour, D.; Laforge, B.; Laplace, S.; Lavrijsen, W.; Le Dortz, O.; Lefebvre, G.; Solis, A. Lopez; Luzi, P. M.; Malaescu, B.; Marchiori, G.; Nikolic-Audit, I.; Ocariz, J.; Pandini, C. E.; Pires, S.; Ridel, M.; Roos, L.; Trincaz-Duvoid, S.; Varouchas, D.; Yap, Y. C.] CNRS IN2P3, Paris, France.
[Akesson, T. P. A.; Bocchetta, S. S.; Bryngemark, L.; Doglioni, C.; Floderus, A.; Hedberg, V.; Jarlskog, G.; Lytken, E.; Mjoernmark, J. U.; Smirnova, O.; Viazlo, O.] Lund Univ, Fys Inst, Lund, Sweden.
[Barreiro, F.; De la Torre, H.; Del Peso, J.; Glasman, C.; Terron, J.] Univ Autonoma Madrid, Dept Fis Teor C 15, Madrid, Spain.
[Artz, S.; Becker, M.; Bertella, C.; Blum, W.; Buescher, V.; Caputo, R.; Caudron, J.; Cuth, J.; Endner, O. C.; Ertel, E.; Fiedler, F.; Torregrosa, E. Fullana; Geisen, M.; Groh, S.; Heck, T.; Jakobi, K. B.; Kaluza, A.; Karnevskiy, M.; Kleinknecht, K.; Koepke, L.; Lin, T. H.; Masetti, L.; Mattmann, J.; Meyer, C.; Moritz, S.; Pleskot, V.; Rave, S.; Sander, H. G.; Schaeffer, J.; Schafer, U.; Schmitt, C.; Schmitz, S.; Schott, M.; Schuh, N.; Simioni, E.; Simon, M.; Tapprogge, S.; Urrejola, P.; Webb, S.; Yildirim, E.; Zimmermann, C.; Zinser, M.] Johannes Gutenberg Univ Mainz, Inst Phys, Mainz, Germany.
[Barnes, S. L.; Bielski, R.; Cox, B. E.; Da Via, C.; Dann, N. S.; Forcolin, G. T.; Forti, A.; Ponce, J. M. Iturbe; Li, X.; Loebinger, F. K.; Mann, A; Marsden, S. P.; Masik, J.; Sanchez, F. J. Munoz; Neep, T. J.; Oh, A.; Ospanov, R.; Pater, J. R.; Peters, R. F. Y.; Pilkington, A. D.; Pin, A. W. J.; Price, D.; Qin, Y.; Queitsch-Maitland, M.; Raine, J. A.; Schweiger, H.; Shaw, S. M.; Tomlinson, L.; Watts, S.; Wilk, F.; Woudstra, M. J.; Wyatt, T. R.] Univ Manchester, Sch Phys & Astron, Manchester, Lancs, England.
[Aad, G.; Alstaty, M.; Barbero, M.; Calandri, A.; Calvet, T. P.; Coadou, Y.; Diaconu, C.; Diglio, S.; Djama, F.; Ellajosyula, V.; Feligioni, L.; Hadef, A.; Hallewell, G. D.; Hubaut, F.; Kahn, S. J.; Knoops, E. B. F. G.; Le Guirriec, E.; Liu, J.; Liu, K.; Madaffari, D.; Mann, A; Monnier, E.; Muanza, S.; Nagy, E.; Pralavorio, P.; Rodina, Y.; Rozanov, A.; Talby, M.; Theveneaux-Pelzer, T.; Torres, R. E. Ticse; Tisserant, S.; Toth, J.; Touchard, F.; Vacavant, L.; Wang, C.] Aix Marseille Univ, CPPM, Marseille, France.
[Aad, G.; Aloisio, A.; Alonso, A.; Alstaty, M.; Barbero, M.; Calandri, A.; Calvet, T. P.; Coadou, Y.; Diaconu, C.; Diglio, S.; Djama, F.; Ellajosyula, V.; Feligioni, L.; Hadef, A.; Hallewell, G. D.; Hubaut, F.; Kahn, S. J.; Knoops, E. B. F. G.; Le Guirriec, E.; Liu, J.; Liu, K.; Madaffari, D.; Mann, A; Monnier, E.; Muanza, S.; Nagy, E.; Pralavorio, P.; Rodina, Y.; Rozanov, A.; Talby, M.; Theveneaux-Pelzer, T.; Torres, R. E. Ticse; Tisserant, S.; Toth, J.; Touchard, F.; Vacavant, L.; Wang, C.] CNRS IN2P3, Marseille, France.
[Bellomo, M.; Bernard, N. R.; Brau, B.; Dallapiccola, C.; Daya-Ishmukhametova, R. K.; Moyse, E. J. W.; Pais, P.; Pettersson, N. E.; Picazio, A.; Willocq, S.] Univ Massachusetts, Dept Phys, Amherst, MA 01003 USA.
[Belanger-Champagne, C.; Chuinard, A. J.; Corriveau, F.; Keyes, R. A.; Mantifel, R.; Prince, S.; Robertson, S. H.; Robichaud-Veronneau, A.; Stockton, M. C.; Stoebe, M.; Vachon, B.; Schroeder, T. Vazquez; Wang, K.; Warburton, A.] McGill Univ, Dept Phys, Montreal, PQ, Canada.
[Barberio, E. L.; Brennan, A. J.; Dawe, E.; Goldfarb, S.; Jennens, D.; Kubota, T.; Le, B.; McDonald, E. F.; Milesi, M.; Nuti, F.; Rados, P.; Scutti, F.; Spiller, L. A.; Tan, K. G.; Taylor, G. N.; Taylor, P. T. E.; Ungaro, F. C.; Urquijo, P.; Volpi, M.; Zanzi, D.] Univ Melbourne, Sch Phys, Melbourne, Vic, Australia.
[Amidei, D.; Chelstowska, M. A.; Cheng, H. C.; Dai, T.; Diehl, E. B.; Edgar, R. C.; Feng, H.; Ferretti, C.; Fleischmann, P.; Guan, L.; Levin, D.; Liu, H.; Lu, N.; Marley, D. E.; Mc Kee, S. P.; McCarn, A.; Neal, H. A.; Qian, J.; Schwarz, T. A.; Searcy, J.; Sekhon, K.; Wu, Y.; Yu, J. M.; Zhang, D.; Zhou, B.; Zhu, J.] Univ Michigan, Dept Phys, Ann Arbor, MI 48109 USA.
[Arabidze, G.; Brock, R.; Chegwidden, A.; Fisher, W. C.; Halladjian, G.; Hauser, R.; Hayden, D.; Huston, J.; Martin, B.; Mondragon, M. C.; Plucinski, P.; Pope, B. G.; Schoenrock, B. D.; Schwienhorst, R.; Willis, C.] Michigan State Univ, Dept Phys & Astron, E Lansing, MI 48824 USA.
[Alimonti, G.; Andreazza, A.; Carminati, L.; Cavalli, D.; Citterio, M.; Costa, G.; Fanti, M.; Giugni, D.; Lazzaroni, M.; Mandelli, L.; Manzoni, S.; Mazza, S. M.; Meroni, C.; Monzani, S.; Perini, L.; Ragusa, F.; Ratti, M. G.; Resconi, S.; Shojaii, S.; Stabile, A.; Tartarelli, G. F.; Troncon, C.; Turra, R.; Perez, M. Villaplana] Univ Milan, Sez Milano, Ist Nazl Fis Nucl, Milan, Italy.
[Andreazza, A.; Carminati, L.; Fanti, M.; Lazzaroni, M.; Manzoni, S.; Mazza, S. M.; Monzani, S.; Perini, L.; Ragusa, F.; Ratti, M. G.; Shojaii, S.; Turra, R.; Perez, M. Villaplana] Univ Milan, Dipartimento Fis, Milan, Italy.
[Harkusha, S.; Kulchitsky, Y.; Kurochkin, Y. A.; Tsiareshka, P. V.] Natl Acad Sci Belarus, BI Stepanov Inst Phys, Minsk, Byelarus.
[Hrynevich, A.] Natl Sci & Educ Ctr Particle & High Energy Phys, Minsk, Byelarus.
[Arguin, J-F.; Azuelos, G.; Dallaire, F.; Ducu, O. A.; Gagnon, L. G.; Gauthier, L.; Leroy, C.; Mann, A; Mochizuki, K.; Manh, T. Nguyen; Rezvani, R.; Saadi, D. Shoaleh] Univ Montreal, Grp Particle Phys, Montreal, PQ, Canada.
[Akimov, A. V.; Gavrilenko, I. L.; Komar, A. A.; Mashinistov, R.; Mouraviev, S. V.; Nechaeva, P. Yu.; Shmeleva, A.; Snesarev, A. A.; Sulin, V. V.; Tikhomirov, V. O.; Zhukov, K.] Russian Acad Sci, PN Lebedev Phys Inst, Moscow, Russia.
[Artamonov, A.; Gorbounov, P. A.; Khovanskiy, V.; Shatalov, P. B.; Tsukerman, I. I.] Inst Theoret & Expt Phys ITEP, Moscow, Russia.
[Artamonov, A.; Gorbounov, P. A.; Khovanskiy, V.; Shatalov, P. B.; Tsukerman, I. I.] Natl Res Nucl Univ MEPhI, Moscow, Russia.
[Antonov, A.; Belotskiy, K.; Belyaev, N. L.; Bulekov, O.; Dolgoshein, B. A.; Kantserov, V. A.; Krasnopevtsev, D.; Mann, A; Romaniouk, A.; Shulga, E.; Smirnov, S. Yu.; Smirnov, Y.; Soldatov, E. Yu.; Timoshenko, S.; Vorobev, K.] Natl Res Nucl Univ MEPhI, Moscow, Russia.
[Gladilin, L. K.; Kramarenko, V. A.; Maevskiy, A.; Sivoklokov, S. Yu.; Smirnova, L. N.; Turchikhin, S.] Moscow MV Lomonosov State Univ, DV Skobeltsyn Inst Nucl Phys, Moscow, Russia.
[Bock, C.; Chow, B. K. B.; Duckeck, G.; Hoenig, F.; Legger, F.; Lorenz, J.; Mann, A; Meineck, C.; Mitrevski, J. .; Rauscher, F.; Ruschke, A.; Schachtner, B. M.; Schaile, D.; Unverdorben, C.; Valderanis, C.] Ludwig Maximilians Univ Munchen, Fak Phys, Munich, Germany.
[Barillari, T.; Bethke, S.; Compostella, G.; Cortiana, G.; Ecker, K. M.; Flowerdew, M. J.; Giuliani, C.; Goblirsch-Kolb, M.; Ince, T.; Kiryunin, A. E.; Kluth, S.; Kortner, O.; Kortner, S.; Kroha, H.; La Rosa, A.; Macchiolo, A.; Maier, A. A.; McCarthy, T. G.; Menke, S.; Mueller, F.; Nisius, R.; Nowak, S.; Oberlack, H.; Richter, R.; Salihagic, D.; Sandstroem, R.; Schacht, P.; Schmidt-Sommerfeld, K. R.; Schwegler, Ph.; Spettel, F.; Stonjek, S.; Terzo, S.; von der Schmitt, H.; Wildauer, A.] Werner Heisenberg Inst, Max Planck Inst Phys, Munich, Germany.
[Fusayasu, T.; Shimojima, M.] Nagasaki Inst Appl Sci, Nagasaki, Japan.
[Horii, Y.; Kentaro, K.; Onogi, K.; Tomoto, M.; Wakabayashi, J.; Yamauchi, K.] Nagoya Univ, Grad Sch Sci, Nagoya, Aichi, Japan.
[Horii, Y.; Kentaro, K.; Onogi, K.; Tomoto, M.; Wakabayashi, J.; Yamauchi, K.] Nagoya Univ, Kobayashi Maskawa Inst, Nagoya, Aichi, Japan.
[Aloisio, A.; Alviggi, M. G.; Canale, V.; Carlino, G.; Cirotto, F.; Conventi, F.; De Asmundis, R.; Della Pietra, M.; Doria, A.; Izzo, V.; Merola, L.; Perrella, S.; Rossi, E.; Sanchez, A.; Sekhniaidze, G.] Univ Napoli, Ist Nazl Fis Nucl, Sez Napoli, Naples, Italy.
[Aloisio, A.; Alviggi, M. G.; Canale, V.; Cirotto, F.; Merola, L.; Perrella, S.; Rossi, E.; Sanchez, A.] Univ Napoli, Dipartimento Fis, Naples, Italy.
[Gorelov, I.; Hoeferkamp, M. R.; Mc Fadden, N. C.; Seidel, S. C.; Taylor, A. C.; Toms, K.] Univ New Mexico, Dept Phys & Astron, Albuquerque, NM 87131 USA.
[Caron, S.; Colasurdo, L.; Croft, V.; De Groot, N.; Filthaut, F.; Galea, C.; Koenig, A. C.; Nektarijevic, S.; Strubig, A.] Radboud Univ Nijmegen Nikhef, Inst Math Astrophys & Particle Phys, Nijmegen, Netherlands.
[Aben, R.; Angelozzi, I.; Bedognetti, M.; Beemster, L. J.; Bentvelsen, S.; Berge, D.; Bobbink, G. J.; Bos, K.; Brenner, L.; Bruni, L. S.; Butti, P.; Castelijn, R.; Castelli, A.; Colijn, A. P.; de Jong, P.; Deigaard, I.; Duda, D.; Ferrari, P.; Hartjes, F.; Hessey, N. P.; Igonkina, O.; Kluit, P.; Koffeman, E.; Mahlstedt, J.; Meyer, J.; Oussoren, K. P.; Sabato, G.; Salek, D.; Slawinska, M.; Valencic, N.; Van Den Wollenberg, W.; Van Der Deij, P. C.; Van der Geer, R.; van der Graaf, H.; van Vulpen, I.; Vankov, P.; Verkerke, W.; Vermeulen, J. C.; Vreeswijk, M.; Weits, H.; Williams, S.] Nikhef Natl Inst Subat Phys, Amsterdam, Netherlands.
[Aben, R.; Angelozzi, I.; Bedognetti, M.; Beemster, L. J.; Bentvelsen, S.; Berge, D.; Bobbink, G. J.; Bos, K.; Brenner, L.; Bruni, L. S.; Butti, P.; Castelijn, R.; Castelli, A.; Colijn, A. P.; de Jong, P.; Deigaard, I.; Duda, D.; Ferrari, P.; Hartjes, F.; Hessey, N. P.; Igonkina, O.; Kluit, P.; Koffeman, E.; Mahlstedt, J.; Meyer, J.; Oussoren, K. P.; Sabato, G.; Salek, D.; Slawinska, M.; Valencic, N.; Van Den Wollenberg, W.; Van Der Deij, P. C.; Van der Geer, R.; van der Graaf, H.; van Vulpen, I.; Vankov, P.; Verkerke, W.; Vermeulen, J. C.; Vreeswijk, M.; Weits, H.; Williams, S.] Univ Amsterdam, Amsterdam, Netherlands.
[Adelman, J.; Andari, N.; Burghgrave, B.; Chakraborty, D.; Klimek, P.; Saha, P.] Univ Illinois, Dept Phys, De Kalb, IL USA.
[Anisenkov, A. V.; Baldin, E. M.; Bobrovnikov, V. S.; Bogdanchikov, A. G.; Buzykaev, A. R.; Kazanin, V. F.; Kharlamov, A. G.; Korol, A. A.; Maslennikov, A. L.; Maximov, D. A.; Peleganchuk, S. V.; Rezanova, O. L.; Soukharev, A. M.; Talyshev, A. A.; Tikhonov, Yu. A.] SB RAS, Budker Inst Nucl Phys, Novosibirsk, Russia.
[Becot, C.; Bernius, C.; Cranmer, K.; Haas, A.; Heinrich, L.; Kaplan, B.; Karthik, K.; Konoplich, R.; Mincer, A. I.; Nemethy, P.; Neves, R. M.] NYU, Dept Phys, 4 Washington Pl, New York, NY 10003 USA.
[Beacham, J. B.; Che, S.; Gan, K. K.; Ishmukhametov, R.; Kagan, H.; Kass, R. D.; Looper, K. A.; Shrestha, S.; Tannenwald, B. B.] Ohio State Univ, Columbus, OH 43210 USA.
[Nakano, I.] Okayama Univ, Fac Sci, Okayama, Japan.
[Abbott, B.; Alhroob, M.; Bertsche, D.; De Benedetti, A.; Gutierrez, R.; Hasib, A.; Norberg, S.; Pearson, B.; Rifki, O.; Severini, H.; Skubic, P.; Strauss, M.] Univ Oklahoma, Homer L Dodge Dept Phys & Astron, Norman, OK 73019 USA.
[Cantero, J.; Haley, J.; Jamin, D. O.; Khanov, A.; Rizatdinova, F.; Sidorov, D.] Oklahoma State Univ, Dept Phys, Stillwater, OK 74078 USA.
[Chytka, L.; Hamal, P.; Hrabovsky, M.; Kvita, J.; Nozka, L.] Palacky Univ, RCPTM, Olomouc, Czech Republic.
[Abreu, R.; Allen, B. W.; Brau, J. E.; Brost, E.; Hopkins, W. H.; Majewski, S.; Potter, C. T.; Radloff, P.; Sinev, N. B.; Strom, D. M.; Torrence, E.; Wanotayaroj, C.; Whalen, K.; Winklmeier, F.] Univ Oregon, Ctr High Energy Phys, Eugene, OR 97403 USA.
[Abeloos, B.; Ayoub, M. K.; Bassalat, A.; Binet, S.; Bourdarios, C.; De Regie, J. B. De Vivie; Delgove, D.; Duflot, L.; Escalier, M.; Fayard, L.; Fournier, D.; Gkougkousis, E. L.; Goudet, C. R.; Grivaz, J. -F.; Hariri, F.; Henrot-Versille, S.; Hrivnac, J.; Iconomidou-Fayard, L.; Kado, M.; Lounis, A.; Maiani, C.; Makovec, N.; Morange, N.; Nellist, C.; Petroff, P.; Poggioli, L.; Puzo, P.; Rousseau, D.; Rybkin, G.; Schaffer, A. C.; Serin, L.; Simion, S.; Tanaka, R.; Zerwas, D.; Zhang, Z.] Univ Paris Saclay, Univ Paris Sud, LAL, CNRS IN2P3, Orsay, France.
[Endo, M.; Nomachi, M.; Sugaya, Y.; Teoh, J. J.; Yamaguchi, Y.] Osaka Univ, Grad Sch Sci, Osaka, Japan.
[Bugge, M. K.; Cameron, D.; Catmore, J. R.; Feigl, S.; Franconi, L.; Garonne, V.; Gjelsten, B. K.; Gramstad, E.; Mann, A; Morisbak, V.; Nilsen, J. K.; Ould-Saada, F.; Pajchel, K.; Pedersen, M.; Raddum, S.; Read, A. L.; Rohne, O.; Sandaker, H.; Serfon, C.; Stapnes, S.; Strandlie, A.] Univ Oslo, Dept Phys, Oslo, Norway.
[Artoni, G.; Barr, A. J.; Becker, K.; Beresford, L.; Bortoletto, D.; Burr, J. T. P.; Cooper-Sarkar, A. M.; Frost, J. A.; Gallas, E. J.; Giuli, F.; Gwenlan, C.; Hays, C. P.; Henderson, J.; Issever, C.; Kalderon, C. W.; Mann, A; Nagai, K.; Tseng, J. C-L.; Viehhauser, G. H. A.; Vigani, L.; Weidberg, A. R.; Zhong, J.] Univ Oxford, Dept Phys, Oxford, England.
[Dondero, P.; Ferrari, R.; Fraternali, M.; Gaudio, G.; Introzzi, G.; Lanza, A.; Laurelli, P.; Livan, M.; Negri, A.; Polesello, G.; Rebuzzi, D. M.; Rimoldi, A.; Vercesi, V.] Univ Pavia, Ist Nazl Fis Nucl, Sez Pavia, Pavia, Italy.
[Dondero, P.; Fraternali, M.; Introzzi, G.; Livan, M.; Negri, A.; Rebuzzi, D. M.; Rimoldi, A.] Univ Pavia, Dipartimento Fis, Pavia, Italy.
[Balunas, W. K.; Brendlinger, K.; Di Clemente, W. K.; Fletcher, R. R. M.; Haney, B.; Heim, S.; Hines, E.; Jackson, B.; Kroll, J.; Lipeles, E.; Miguens, J. Machado; Meyer, C.; Mistry, K. P.; Reichert, J.; Thomson, E.; Vanguri, R.; Williams, H. H.; Yoshihara, K.] Univ Penn, Dept Phys, Philadelphia, PA 19104 USA.
[Basalaev, A.; Ezhilov, A.; Fedin, O. L.; Gratchev, V.; Levchenko, M.; Maleev, V. P.; Naryshkin, I.; Ryabov, Y. F.; Schegelsky, V. A.; Seliverstov, D. M.; Solovyev, V.] BP Konstantinov Petersburg Nucl Phys Inst, Kurchatov Inst, Natl Res Ctr, St Petersburg, Russia.
[Aloisio, A.; Annovi, A.; Bertolucci, F.; Biesuz, N. V.; Cavasinni, V.; Chiarelli, G.; Del Prete, T.; Dell'Orso, M.; Donati, S.; Giannetti, P.; Leone, S.; Mann, A; Roda, C.; Scuri, F.; Sotiropoulou, C. L.; Spalla, M.; Volpi, G.] Univ Pisa, Ist Nazl Fis Nucl, Sez Pisa, Pisa, Italy.
[Annovi, A.; Bertolucci, F.; Biesuz, N. V.; Cavasinni, V.; Chiarelli, G.; Del Prete, T.; Dell'Orso, M.; Donati, S.; Giannetti, P.; Leone, S.; Mann, A; Roda, C.; Scuri, F.; Sotiropoulou, C. L.; Spalla, M.; Volpi, G.] Univ Pisa, Dipartimento Fis E Fermi, Pisa, Italy.
[Bianchi, R. M.; Boudreau, J.; Escobar, C.; Farina, C.; Hong, T. M.; Mueller, J.; Sapp, K.; Su, J.] Univ Pittsburgh, Dept Phys & Astron, Pittsburgh, PA 15260 USA.
[Aguilar-Saavedra, J. A.; Dos Santos, S. P. Amor; Amorim, A.; Araque, J. P.; Cantrill, R.; Carvalho, J.; Castro, N. F.; Muino, R. Conde; De Sousa, M. J. Da Cunha Sargedas; Fiolhais, M. C. N.; Galhardo, B.; Glazov, A.; Gomes, A.; Goncalo, R.; Jorge, P. M.; Lopes, L.; Maio, A.; Maneira, J.; Mann, A; Seabra, L. F. Oleiro; Onofre, A.; Palma, A.; Pedro, R.; Santos, H.; Saraiva, J. G.; Silva, J.; Delgado, A. Tavares; Veloso, F.; Wolters, H.] LIP, Lab Instrumentacao & Fis Expt Particulas, Lisbon, Portugal.
[Amorim, A.; Muino, R. Conde; De Sousa, M. J. Da Cunha Sargedas; Glazov, A.; Gomes, A.; Jorge, P. M.; Miguens, J. Machado; Maio, A.; Maneira, J.; Mann, A; Palma, A.; Pedro, R.; Delgado, A. Tavares] Univ Lisbon, Fac Ciencias, Lisbon, Portugal.
[Dos Santos, S. P. Amor; Carvalho, J.; Fiolhais, M. C. N.; Galhardo, B.; Onofre, A.; Veloso, F.; Wolters, H.] Univ Coimbra, Dept Phys, Coimbra, Portugal.
[Gomes, A.; Maio, A.; Saraiva, J. G.; Silva, J.] Univ Lisbon, Ctr Fis Nucl, Lisbon, Portugal.
Univ Minho, Dept Fis, Braga, Portugal.
[Aguilar-Saavedra, J. A.; Glazov, A.] Univ Granada, Dept Fis Teor & Cosmos, Granada, Spain.
Univ Granada, CAFPE, Granada, Spain.
Univ Nova Lisboa, Fac Ciencias & Tecnol, Dep Fis & CEFITEC, Caparica, Portugal.
[Chudoba, J.; Havranek, M.; Hejbal, J.; Jakoubek, T.; Kepka, O.; Kupco, A.; Kus, V.; Lokajicek, M.; Lysak, R.; Marcisovsky, M.; Mikestikova, M.; Nemecek, S.; Penc, O.; Sicho, P.; Staroba, P.; Svatos, M.; Tasevsky, M.; Vrba, V.] Acad Sci Czech Republic, Inst Phys, Prague, Czech Republic.
[Ali, B.; Augsten, K.; Caforio, D.; Gallus, P.; Hubacek, Z.; Myska, M.; Pospisil, S.; Seifert, F.; Simak, V.; Slavicek, T.; Smolek, K.; Solar, M.; Sopczak, A.; Sopko, V.; Suk, M.; Turecek, D.; Vacek, V.; Vlasak, M.; Vokac, P.; Vykydal, Z.; Zeman, M.] Czech Tech Univ, Prague, Czech Republic.
[Balek, P.; Berta, P.; Carli, I.; Davidek, T.; Dolejsi, J.; Dolezal, Z.; Kodys, P.; Kosek, T.; Leitner, R.; Reznicek, P.; Scheirich, D.; Slovak, R.; Spousta, M.; Sykora, T.; Tas, P.; Todorova-Nova, S.; Valkar, S.; Vorobel, V.] Charles Univ Prague, Fac Math & Phys, Prague, Czech Republic.
[Borisov, A.; Cheremushkina, E.; Denisov, S. P.; Fakhrutdinov, R. M.; Fenyuk, A. B.; Golubkov, D.; Kamenshchikov, A.; Karyukhin, A. N.; Kozhin, A. S.; Mann, A; Minaenko, A. A.; Myagkov, A. G.; Nikolaenko, V.; Ryzhov, A.; Solodkov, A. A.; Solovyanov, O. V.; Starchenko, E. A.; Vaniachine, A.; Zaitsev, A. M.; Zenin, O.] NRC KI, State Res Ctr Inst High Energy Phys, Protvino, Russia.
[Adye, T.; Baines, J. T.; Barnett, B. M.; Burke, S.; Dewhurst, A.; Dopke, J.; Emeliyanov, D.; Gallop, B. J.; Gee, C. N. P.; Haywood, S. J.; Kirk, J.; Martin-Haugh, S.; McMahon, S. J.; Middleton, R. P.; Murray, W. J.; Phillips, P. W.; Sankey, D. P. C.; Sawyer, C.; Tyndel, M.; Wickens, F. J.; Wielers, M.; Worm, S. D.] Rutherford Appleton Lab, Particle Phys Dept, Didcot, Oxon, England.
[Aloisio, A.; Alonso, A.; Anulli, F.; Bagiacchi, P.; Bagnaia, P.; Bauce, M.; Bini, C.; Ciapetti, G.; Corradi, M.; De Pedis, D.; De Salvo, A.; Di Donato, C.; Falciano, S.; Gentile, S.; Giagu, S.; Gustavino, G.; Kuna, M.; Lacava, F.; Luci, C.; Luminari, L.; Mann, A; Messina, A.; Nisati, A.; Pasqualucci, E.; Petrolo, E.; Pontecorvo, L.; Rescigno, M.; Rosati, S.; Tehrani, F. Safai; Vanadia, M.; Vari, R.; Veneziano, S.; Verducci, M.; Zanello, L.] Sapienza Univ Roma, Sez Roma, Ist Nazl Fis Nucl, Rome, Italy.
[Bagiacchi, P.; Bagnaia, P.; Bauce, M.; Bini, C.; Ciapetti, G.; Corradi, M.; Di Donato, C.; Gentile, S.; Giagu, S.; Gustavino, G.; Kuna, M.; Lacava, F.; Luci, C.; Messina, A.; Vanadia, M.; Verducci, M.; Zanello, L.] Sapienza Univ Roma, Dipartimento Fis, Rome, Italy.
[Aielli, G.; Camarri, P.; Cardarelli, R.; Di Ciaccio, A.; Iuppa, R.; Liberti, B.; Salamon, A.; Santonico, R.] Univ Roma Tor Vergata, Sez Roma Tor Vergata, Ist Nazl Fis Nucl, Rome, Italy.
[Aielli, G.; Camarri, P.; Di Ciaccio, A.; Iuppa, R.; Salamon, A.; Santonico, R.] Univ Roma Tor Vergata, Dipartimento Fis, Rome, Italy.
[Baroncelli, A.; Biglietti, M.; Ceradini, F.; Di Micco, B.; Farilla, A.; Graziani, E.; Iodice, M.; Orestano, D.; Petrucci, F.; Puddu, D.; Salamanna, G.; Sessa, M.; Stanescu, C.; Taccini, C.] Univ Roma Tre, Sez Roma Tre, Ist Nazl Fis Nucl, Rome, Italy.
[Ceradini, F.; Di Micco, B.; Mann, A; Orestano, D.; Petrucci, F.; Puddu, D.; Salamanna, G.; Sessa, M.; Taccini, C.] Univ Roma Tre, Dipartimento Matemat & Fis, Rome, Italy.
[Benchekroun, D.; Chafaq, A.; Hoummada, A.] Univ Hassan 2, Reseau Univ Phys Hautes Energies, Fac Sci Ain Chock, Casablanca, Morocco.
[Ghazlane, H.] Ctr Natl Energie Sci Tech Nucl, Rabat, Morocco.
[El Kacimic, M.; Goujdami, D.] Univ Cadi Ayyad, LPHEA Marrakech, Fac Sci Semlalia, Marrakech, Morocco.
[Aaboud, M.; Derkaoui, J. E.; Ouchrif, M.; Tayalati, Y.] Univ Mohamed Premier, Fac Sci, Oujda, Morocco.
[Aaboud, M.; Derkaoui, J. E.; Ouchrif, M.; Tayalati, Y.] LPTPM, Oujda, Morocco.
[El Moursli, R. Cherkaoui; Fassi, F.; Haddad, N.; Idrissi, Z.] Univ Mohammed 5, Fac Sci, Rabat, Morocco.
[Bachacou, H.; Balli, F.; Bauer, F.; Besson, N.; Blanchard, J. -B.; Boonekamp, M.; Chevalier, L.; Hoffmann, M. Dano; Deliot, F.; Denysiuk, D.; Etienvre, A. I.; Formica, A.; Giraud, P. F.; Da Costa, J. Goncalves Pinto Firmino; Guyot, C.; Hanna, R.; Hassani, S.; Jeanneau, F.; Kivernyk, O.; Kozanecki, W.; Kukla, R.; Lancon, E.; Laporte, J. F.; Laycock, P.; Le Quilleuc, E. P.; Lesage, A. A. J.; Mann, A; Mansoulie, B.; Meyer, J-P.; Nicolaidou, R.; Ouraou, A.; Rodriguez, L. Pacheco; Perego, M. M.; Peyaud, A.; Royon, C. R.; Saimpert, M.; Schoeffel, L.; Schune, Ph.; Schwemling, Ph.; Schwindling, J.] CEA Saclay Commissariat Energie Atom & Energies A, Inst Rech Lois Fondamentales Univers, DSM IRFU, Gif Sur Yvette, France.
[AbouZeid, O. S.; Battaglia, M.; Debenedetti, C.; Grillo, A. A.; Hance, M.; Kuhl, A.; Litke, A. M.; Lockman, W. S.; Nielsen, J.; Reece, R.; Rose, P.; Sadrozinski, H. F-W.; Schier, S.; Schumm, B. A.; Seiden, A.] Univ Calif Santa Cruz, Santa Cruz Inst Particle Phys, Santa Cruz, CA 95064 USA.
[Alpigiani, C.; Blackburn, D.; Goussiou, A. G.; Hsu, S. -C.; Johnson, W. J.; Lubattin, H. J.; Marx, M.; Meehan, S.; Rompotis, N.; Rosten, R.; Rothberg, J.; Russell, H. L.; De Bruin, P. H. Sales; Pastor, E. Torro; Watts, G.; Whallon, N. L.] Univ Washington, Dept Phys, Seattle, WA 98195 USA.
[Anastopoulos, C.; Costanzo, D.; Dawson, I.; Fletcher, G. T.; Hamity, G. N.; Klinger, J. A.; Korolkova, E. V.; Kyriazopoulos, D.; Paredes, B. Lopez; Macdonald, C. M.; Mann, A; Tovey, D. R.] Univ Sheffield, Dept Phys & Astron, Sheffield, S Yorkshire, England.
[Hasegawa, Y.; Takeshita, T.] Shinshu Univ, Dept Phys, Nagano, Japan.
[Atlay, N. B.; Buchholz, P.; Campoverde, A.; Czirr, H.; Fleck, I.; Gaur, B.; Ghasemi, S.; Ibragimov, I.; Li, Y.; Rosenthal, O.; Walkowiak, W.; Ziolkowski, M.] Univ Siegen, Fachbereich Phys, Siegen, Germany.
[Buat, Q.; Horton, A. J.; Mori, D.; O'Neil, D. C.; Pachal, K.; Stelzer, B.; Temple, D.; Torres, H.; Van Nieuwkoop, J.; Vetterli, M. C.] Simon Fraser Univ, Dept Phys, Burnaby, BC, Canada.
[Armbruster, A. J.; Bawa, H. S.; Black, J. E.; Garelli, N.; Grenier, P.; Ilic, N.; Kagan, M.; Kocian, M.; Malone, C.; Mann, A; Moss, J.; Nachman, B. P.; Piacquadio, G.; Rubbo, F.; Salnikov, A.; Schwartzman, A.; Su, D.; Tompkins, L.; Wittgen, M.; Young, C.] SLAC Natl Accelerator Lab, Stanford, CA USA.
[Astalos, R.; Bartos, P.; Blazek, T.; Dado, T.; Mann, A; Melo, M.; Plazak, L.; Smiesko, J.; Sykora, I.; Tokar, S.; Zenis, T.] Comenius Univ, Fac Math Phys & Informat, Bratislava, Slovakia.
[Bruncko, D.; Kladiva, E.; Strizenec, P.; Urban, J.] Slovak Acad Sci, Inst Expt Phys, Dept Subnucl Phys, Kosice, Slovakia.
[Castaneda-Miranda, E.; Hamilton, A.; Yacoob, S.] Univ Cape Town, Dept Phys, Cape Town, South Africa.
[Connell, S. H.; Govender, N.] Univ Johannesburg, Dept Phys, Johannesburg, South Africa.
[Hsu, C.; Kar, D.; Garcia, B. R. Mellado; Ruan, X.] Univ Witwatersrand, Sch Phys, Johannesburg, South Africa.
[Akerstedt, H.; Asman, B.; Bendtz, K.; Bertoli, G.; Bylund, O. Bessidskaia; Bohm, C.; Clement, C.; Cribbs, W. A.; Hellman, S.; Jon-And, K.; Lundberg, O.; Milstead, D. A.; Moa, T.; Molander, S.; Pani, P.; Poettgen, R.; Rossetti, V.; Shaikh, N. W.; Shcherbakova, A.; Silverstein, S. B.; Sjolin, J.; Strandberg, S.; Ughetto, M.; Santurio, E. Valdes; Wallangen, V.] Stockholm Univ, Dept Phys, Stockholm, Sweden.
[Abulaiti, Y.; Akerstedt, H.; Asman, B.; Bendtz, K.; Bertoli, G.; Bylund, O. Bessidskaia; Clement, C.; Cribbs, W. A.; Hellman, S.; Jon-And, K.; Lundberg, O.; Milstead, D. A.; Moa, T.; Molander, S.; Pani, P.; Poettgen, R.; Rossetti, V.; Shaikh, N. W.; Shcherbakova, A.; Sjolin, J.; Strandberg, S.; Ughetto, M.; Santurio, E. Valdes; Wallangen, V.] Oskar Klein Ctr, Stockholm, Sweden.
[Lund-Jensen, B.; Sidebo, P. E.; Strandberg, J.] Royal Inst Technol, Dept Phys, Stockholm, Sweden.
[Balestri, T.; Bee, C. P.; Chen, K.; Hobbs, J.; Huo, R.; Jia, J.; Li, H.; Lindquist, B. E.; McCarthy, R. L.; Montalbano, A.; Morvaj, L.; Radhakrishnan, S. K.; Rijssenbeek, M.; Schamberger, R. D.; Tsybychev, D.; Zaman, A.; Zhou, M.] SUNY Stony Brook, Dept Phys & Astron, Stony Brook, NY 11794 USA.
[Balestri, T.; Bee, C. P.; Chen, K.; Hobbs, J.; Huo, R.; Jia, J.; Li, H.; Lindquist, B. E.; McCarthy, R. L.; Montalbano, A.; Morvaj, L.; Radhakrishnan, S. K.; Rijssenbeek, M.; Schamberger, R. D.; Tsybychev, D.; Zaman, A.; Zhou, M.] SUNY Stony Brook, Dept Chem, Stony Brook, NY 11794 USA.
[Abraham, N. L.; Allbrooke, B. M. M.; Asquith, L.; Cerri, A.; Barajas, C. A. Chavez; De Sanctis, U.; De Santo, A.; Grout, Z. J.; Lerner, G.; Mann, A; Miano, F.; Salvatore, F.; Castillo, I. Santoyo; Shehu, C. Y.; Suruliz, K.; Sutton, M. R.; Vivarelli, I.; Winston, O. J.] Univ Sussex, Dept Phys & Astron, Brighton, E Sussex, England.
[Black, C. W.; Cuthbert, C.; Finelli, K. D.; Jeng, G. -Y.; Limosani, A.; Morley, A. K.; Saavedra, A. F.; Scarcella, M.; Varvell, K. E.; Wang, J.; Yabsley, B.] Univ Sydney, Sch Phys, Sydney, NSW, Australia.
[Hou, S.; Hsu, P. J.; Lee, S. C.; Lin, S. C.; Liu, B.; Liu, D.; Lo Sterzo, F.; Mazini, R.; Shi, L.; Soh, D. A.; Teng, P. K.; Wang, S. M.; Yang, Y.] Acad Sinica, Inst Phys, Taipei, Taiwan.
[Abreu, H.; Gozani, E.; Rozen, Y.; Tarem, S.; van Eldik, N.] Technion Israel Inst Technol, Dept Phys, Haifa, Israel.
[Abramowicz, H.; Alexander, G.; Ashkenazi, A.; Bella, G.; Benary, O.; Benhammou, Y.; Davies, M.; Duarte-Campderros, J.; Etzion, E.; Gershon, A.; Gueta, O.; Oren, Y.; Soffer, A.; Taiblum, N.] Tel Aviv Univ, Raymond & Beverly Sackler Sch Phys & Astron, Tel Aviv, Israel.
[Gkaitatzis, S.; Gkialas, I.; Iliadis, D.; Kimura, N.; Kordas, K.; Kourkoumeli-Charalampidi, A.; Leisos, A.; Papageorgiou, K.; Petridou, C.; Sampsonidis, D.] Aristotle Univ Thessaloniki, Dept Phys, Thessaloniki, Greece.
[Asai, S.; Chen, S.; Dohmae, T.; Enari, Y.; Hanawa, K.; Kanaya, N.; Kataoka, Y.; Kato, C.; Kawamoto, T.; Kazama, S.; Kobayashi, A.; Kobayashi, T.; Komori, Y.; Kozakai, C.; Mashimo, T.; Masubuchi, T.; Minami, Y.; Mori, T.; Morinaga, M.; Nakamura, T.; Ninomiya, Y.; Nobe, T.; Saito, T.; Sakamoto, H.; Sasaki, Y.; Tanaka, J.; Terashi, K.; Ueda, I.; Yamamoto, S.; Yamanaka, T.] Univ Tokyo, Int Ctr Elementary Particle Phys, Tokyo, Japan.
[Asai, S.; Chen, S.; Dohmae, T.; Enari, Y.; Hanawa, K.; Kanaya, N.; Kataoka, Y.; Kato, C.; Kawamoto, T.; Kazama, S.; Kobayashi, A.; Kobayashi, T.; Komori, Y.; Kozakai, C.; Mashimo, T.; Masubuchi, T.; Minami, Y.; Mori, T.; Morinaga, M.; Nakamura, T.; Ninomiya, Y.; Nobe, T.; Saito, T.; Sakamoto, H.; Sasaki, Y.; Tanaka, J.; Terashi, K.; Ueda, I.; Yamamoto, S.; Yamanaka, T.] Univ Tokyo, Dept Phys, Tokyo, Japan.
[Bratzler, U.; Fukunaga, C.] Tokyo Metropolitan Univ, Grad Sch Sci & Technol, Tokyo, Japan.
[Ishitsuka, M.; Jinnouchi, O.; Kobayashi, D.; Kuze, M.; Motohashi, K.; Todome, K.; Yamaguchi, D.] Tokyo Inst Technol, Dept Phys, Tokyo, Japan.
[Batista, S. J.; Chau, C. C.; Cormier, K. J. R.; DeMarco, D. A.; Di Sipio, R.; Diamond, M.; Keoshkerian, H.; Krieger, P.; Liblong, A.; Mann, A; Mc Goldrick, G.; Orr, R. S.; Pascuzzi, V. R.; Polifka, R.; Rudolph, M. S.; Savard, P.; Sinervo, P.; Taenzer, J.; Teuscher, R. J.; Trischuk, W.; Veloce, L. M.; Venturi, N.] Univ Toronto, Dept Phys, Toronto, ON, Canada.
[Canepa, A.; Chekulaev, S. V.; Hod, N.; Jovicevic, J.; Codina, E. Perez; Schneider, B.; Stelzer-Chilton, O.; Tafirouta, R.; Trigger, I. M.] TRIUMF, Vancouver, BC, Canada.
[Ramos, J. Manjarres; Palacino, G.; Taylor, W.] York Univ, Dept Phys & Astron, Toronto, ON, Canada.
[Hara, K.; Ito, F.; Kasahara, K.; Kim, S. H.; Kiuchi, K.; Mann, A; Nagata, K.; Okawa, H.; Sato, K.; Ukegawa, F.] Univ Tsukuba, Fac Pure & Appl Sci, Tsukuba, Ibaraki, Japan.
[Hara, K.; Ito, F.; Kasahara, K.; Kim, S. H.; Kiuchi, K.; Nagata, K.; Okawa, H.; Sato, K.; Ukegawa, F.] Univ Tsukuba, Ctr Integrated Res Fundamental Sci & Engn, Tsukuba, Ibaraki, Japan.
[Beauchemin, P. H.; Meoni, E.; Sliwa, K.; Son, H.; Wetter, J.] Tufts Univ, Dept Phys & Astron, Medford, MA 02155 USA.
[Casper, D. W.; Corso-Radu, A.; Frate, M.; Guest, D.; Lankford, A. J.; Lari, T.; Mete, A. S.; Nelson, A.; Scannicchio, D. A.; Schernau, M.; Shimmin, C. O.; Taffard, A.; Unel, G.; Whiteson, D.] Univ Calif Irvine, Dept Phys & Astron, Irvine, CA USA.
[Acharya, B. S.; Boldyrev, A. S.; Cobal, M.; Giordani, M. P.; Pinamonti, M.; Quayle, W. B.; Serkin, L.; Shaw, K.; Soualah, R.; Truong, L.] Ist Nazl Fis Nucl, Grp Collegato Udine, Sez Trieste, Udine, Italy.
[Acharya, B. S.; Quayle, W. B.; Serkin, L.; Shaw, K.] Abdus Salaam Int Ctr Theoret Phys, Trieste, Italy.
[Boldyrev, A. S.; Cobal, M.; Pinamonti, M.; Soualah, R.; Truong, L.] Univ Udine, Dipartimento Chim Fis & Ambiente, Udine, Italy.
[Kuutmann, E. Bergeaas; Brenner, R.; Ellert, M.; Ferrari, A.; Maddocks, H. J.; Ohman, H.; Pelikan, D.; Rangel-Smith, C.] Uppsala Univ, Dept Phys & Astron, Uppsala, Sweden.
[Atkinson, M.; Armadans, R. Caminal; Cavaliere, V.; Chang, P.; Errede, S.; Hooberman, B. H.; Khader, M.; Lie, K.; Liss, T. M.; Liu, L.; Long, J. D.; Outschoorn, V. I. Martinez; Neubauer, M. S.; Rybar, M.; Shang, R.; Sickles, A. M.; Vichou, I.; Zeng, J. C.] Univ Illinois, Dept Phys, 1110 W Green St, Urbana, IL 61801 USA.
[Piqueras, D. Alvarez; Navarro, L. Barranco; Alberich, L. Cerda; Ferrer, A.; Fiorini, L.; Fuster, J.; Garcia, C.; Navarro, J. E. Garcia; Higon-Rodriguez, E.; Pena, J. Jimenez; Lacasta, C.; Mamuzic, J.; Melini, D.; Rodriguez, D. Rodriguez; Adam, E. Romero; Ros, E.; Salt, J.; Sanchez, J.; Valero, A.; Ferrer, J. A. Valls] Univ Valencia, Inst Fis Corpuscular IFIC, Valencia, Spain.
[Piqueras, D. Alvarez; Navarro, L. Barranco; Urban, S. Cabrera; Alberich, L. Cerda; Costa, M. J.; Martinez, P. Fernandez; Ferrer, A.; Fiorini, L.; Fuster, J.; Garcia, C.; Navarro, J. E. Garcia; de la Hoz, S. Gonzalez; Higon-Rodriguez, E.; Pena, J. Jimenez; King, M.; Lacasta, C.; Mamuzic, J.; Marti-Garcia, S.; Melini, D.; Lopez, S. Pedraza; Rodriguez, D. Rodriguez; Adam, E. Romero; Ros, E.; Salt, J.; Sanchez, J.; Valero, A.; Ferrer, J. A. Valls; Vos, M.] Univ Valencia, Dept Fis Atom Mol & Nucl, Valencia, Spain.
[Piqueras, D. Alvarez; Navarro, L. Barranco; Urban, S. Cabrera; Gimenez, V. Castillo; Alberich, L. Cerda; Costa, M. J.; Martinez, P. Fernandez; Ferrer, A.; Fiorini, L.; Fuster, J.; Garcia, C.; Navarro, J. E. Garcia; de la Hoz, S. Gonzalez; Jimenez, Y. Hernandez; Higon-Rodriguez, E.; Pena, J. Jimenez; King, M.; Lacasta, C.; Lacuesta, V. R.; Mamuzic, J.; Mann, A; Marti-Garcia, S.; Melini, D.; Mitsou, V. A.; Lopez, S. Pedraza; Rodriguez, D. Rodriguez; Adam, E. Romero; Ros, E.; Salt, J.; Sanchez, J.; Martinez, V. Sanchez; Soldevila, U.; Valero, A.; Ferrer, J. A. Valls; Vos, M.] Univ Valencia, Dept Ingn Elect, Valencia, Spain.
[Piqueras, D. Alvarez; Navarro, L. Barranco; Urban, S. Cabrera; Gimenez, V. Castillo; Alberich, L. Cerda; Costa, M. J.; Martinez, P. Fernandez; Ferrer, A.; Fiorini, L.; Fuster, J.; Garcia, C.; Navarro, J. E. Garcia; de la Hoz, S. Gonzalez; Jimenez, Y. Hernandez; Higon-Rodriguez, E.; Pena, J. Jimenez; King, M.; Lacasta, C.; Lacuesta, V. R.; Mamuzic, J.; Mann, A; Marti-Garcia, S.; Melini, D.; Mitsou, V. A.; Lopez, S. Pedraza; Rodriguez, D. Rodriguez; Adam, E. Romero; Ros, E.; Salt, J.; Sanchez, J.; Martinez, V. Sanchez; Soldevila, U.; Valero, A.; Ferrer, J. A. Valls; Vos, M.] Univ Valencia, Inst Microelect Barcelona IMB CNM, Valencia, Spain.
[Aloisio, A.; Piqueras, D. Alvarez; Navarro, L. Barranco; Urban, S. Cabrera; Gimenez, V. Castillo; Alberich, L. Cerda; Costa, M. J.; Martinez, P. Fernandez; Ferrer, A.; Fiorini, L.; Fuster, J.; Garcia, C.; Navarro, J. E. Garcia; de la Hoz, S. Gonzalez; Jimenez, Y. Hernandez; Higon-Rodriguez, E.; Pena, J. Jimenez; King, M.; Lacasta, C.; Lacuesta, V. R.; Mamuzic, J.; Mann, A; Marti-Garcia, S.; Melini, D.; Mitsou, V. A.; Lopez, S. Pedraza; Rodriguez, D. Rodriguez; Adam, E. Romero; Ros, E.; Salt, J.; Sanchez, J.; Martinez, V. Sanchez; Soldevila, U.; Valero, A.; Ferrer, J. A. Valls; Vos, M.] CSIC, Valencia, Spain.
[Danninger, M.; Fedorko, W.; Gay, C.; Gecse, Z.; Gignac, M.; Henkelmann, S.; King, S. B.; Lister, A.] Univ British Columbia, Dept Phys, Vancouver, BC, Canada.
[Albert, J.; David, C.; Elliot, A. A.; Fincke-Keeler, M.; Hamano, K.; Hill, E.; Keeler, R.; Kowalewski, R.; Kuwertz, E. S.; Kwan, T.; LeBlanc, M.; Lefebvre, M.; Mann, A; McPherson, R. A.; Pearce, J.; Seuster, R.; Sobie, R.; Trovatelli, M.; Venturi, M.] Univ Victoria, Dept Phys & Astron, Victoria, BC, Canada.
[Beckingham, M.; Ennis, J. S.; Farrington, S. M.; Harrison, P. F.; Jeske, C.; Jones, G.; Martin, T. A.; Murray, W. J.; Pianori, E.; Spangenberg, M.] Univ Warwick, Dept Phys, Coventry, W Midlands, England.
[Iizawa, T.; Mitani, T.; Sakurai, Y.; Yorita, K.] Waseda Univ, Tokyo, Japan.
[Bressler, S.; Citron, Z. H.; Duchovni, E.; Dumancic, M.; Gross, E.; Koehler, M. K.; Lellouch, D.; Levinson, L. J.; Mikenberg, G.; Milov, A.; Pitt, M.; Ravinovich, I.; Roth, I.; Schaarschmidt, J.; Smakhtin, V.; Turgeman, D.] Weizmann Inst Sci, Dept Particle Phys, Rehovot, Israel.
[Banerjee, Sw.; Guan, W.; Hard, A. S.; Heng, Y.; Ji, H.; Ju, X.; Kaplan, L. S.; Kashif, L.; Kruse, A.; Ming, Y.; Wang, F.; Wiedenmann, W.; Wu, S. L.; Yang, H.; Zhang, F.; Zobernig, G.] Univ Wisconsin, Dept Phys, 1150 Univ Ave, Madison, WI 53706 USA.
[Kuger, F.; Redelbach, A.; Schreyer, M.; Sidiropoulou, O.; Siragusa, G.; Strohmer, R.; Trefzger, T.; Weber, S. W.; Zibell, A.] Julius Maximilians Univ, Fak Phys & Astron, Wurzburg, Germany.
[Bannoura, A. A. E.; Boerner, D.; Braun, H. M.; Cornelissen, T.; Ellinghaus, F.; Ernis, G.; Fischer, J.; Flick, T.; Gabizon, O.; Gilles, G.; Hamacher, K.; Harenberg, T.; Hirschbuehl, D.; Kersten, S.; Kuechler, J. T.; Mann, A; Maettig, P.; Neumann, M.; Pataraia, S.; Riegel, C. J.; Sandhoff, M.; Tepel, F.; Vogel, M.; Wagner, W.; Zeitnitz, C.] Berg Univ Wuppertal, Fak Math & Nat Wissensch, Fachgrp Phys, Wuppertal, Germany.
[Baker, O. K.; Noccioli, E. Benhar; Cummings, J.; Demers, S.; Ideal, E.; Lagouri, T.; Leister, A. G.; Loginov, A.; Hernandez, D. Paredes; Thomsen, L. A.; Tipton, P.; Vasquez, J. G.; Wang, X.] Yale Univ, Dept Phys, New Haven, CT USA.
[Hakobyan, H.; Vardanyan, G.] Yerevan Phys Inst, Yerevan, Armenia.
[Rahal, G.] IN2P3, Ctr Calcul, Villeurbanne, France.
[Acharya, B. S.; Jackson, P.; Lee, L.; Petridis, A.; White, M. J.] Kings Coll London, Dept Phys, London, England.
[Ahmadov, F.; Bouffard, J.; Ernst, J.; Fischer, A.; Guindon, S.; Huseynov, N.; Jain, V.; Javadov, N.] Azerbaijan Acad Sci, Inst Phys, Baku, Azerbaijan.
[Anisenkov, A. V.; Baldin, E. M.; Bobrovnikov, V. S.; Buzykaev, A. R.; Czodrowski, P.; Dassoulas, J.; Dehghanian, N.; Gingrich, D. M.; Jabbar, S.; Karamaoun, A.; Kazanin, V. F.; Kharlamov, A. G.; Korol, A. A.; Maslennikov, A. L.; Maximov, D. A.; Moore, R. W.; Peleganchuk, S. V.; Pinfold, J. L.; Rezanova, O. L.; Soukharev, A. M.; Talyshev, A. A.; Tikhonov, Yu. A.] Novosibirsk State Univ, Novosibirsk, Russia.
[Aloisio, A.; Anisenkov, A. V.; Baldin, E. M.; Bobrovnikov, V. S.; Buzykaev, A. R.; Czodrowski, P.; Dassoulas, J.; Dehghanian, N.; Gingrich, D. M.; Jabbar, S.; Karamaoun, A.; Kazanin, V. F.; Kharlamov, A. G.; Korol, A. A.; Mann, A; Maslennikov, A. L.; Maximov, D. A.; Moore, R. W.; Peleganchuk, S. V.; Pinfold, J. L.; Rezanova, O. L.; Soukharev, A. M.; Talyshev, A. A.; Tikhonov, Yu. A.] Novosibirsk State Univ, Novosibirsk, Russia.
[Azuelos, G.; Cakira, O.; Ciftci, A. K.; Yildiz, H. Duran; Gingrich, D. M.; Oakham, F. G.; Savard, P.; Sultansoy, S.; Vetterli, M. C.] TRIUMF, Vancouver, BC, Canada.
[Banerjee, Sw.; Berger, N.; Delmastro, M.; Di Ciaccio, L.; Elles, S.; Grevtsov, K.; Guillemin, T.; Hryn'ova, T.; Jezequel, S.; Koletsou, I.; Lafaye, R.; Leveque, J.; Mastrandrea, P.; Sauvage, G.; Sauvan, E.; Simard, O.; Smart, B. H.; Todorov, T.; Wingerter-Seez, I.; Yatsenko, E.] Univ Louisville, Dept Phys & Astron, Louisville, KY 40292 USA.
[Bawa, H. S.; Blair, R. E.; Chekanov, S.; Gao, Y. S.; LeCompte, T.; Love, J.; Malon, D.; Metcalfe, J. .; Nguyen, D. H.; Nodulman, L.; Paramonov, A.; Price, L. E.; Proudfoot, J.; Ryu, S.; Stanek, R. W.; van Gemmeren, P.; Wang, R.; Webster, J. S.; Yoshida, R.; Zhang, J.] Calif State Univ Fresno, Dept Phys, Fresno, CA 93740 USA.
[Beck, H. P.; Cheu, E.; Johns, K. A.; Jones, S.; Lamp, W.; Lei, X.; Leone, R.; Loch, P.; Nayyar, R.; O'grady, F.; Rutherfoord, J. P.; Shupe, M. A.; Varnes, E. W.] Univ Fribourg, Dept Phys, Fribourg, Switzerland.
[Brandt, A.; Bullock, D.; Casado, M. P.; Darmora, S.; De, K.; Farbin, A.; Feremenga, L.; Griffiths, J.; Hadavand, H. K.; Heelan, L.; Kim, H. Y.; Ozturk, N.; Schovancova, J.; Stradling, A. R.; Usai, G.; Vartapetian, A.; White, A.; Yu, J.] Univ Autonoma Barcelona, Dept Fis, Barcelona, Spain.
[Angelidakis, S.; Castro, N. F.; Chouridou, S.; Fassouliotis, D.; Giokaris, N.; Ioannou, P.; Kourkoumelis, C.; Tsirintanis, N.] Univ Porto, Dept Fis & Astron, Fac Ciencias, Oporto, Portugal.
[Alexopoulos, T.; Aloisio, A.; Benekos, N.; Chelkov, G. A.; Dris, M.; Gazis, E. N.; Karakostas, K.; Karastathis, N.; Karentzos, E.; Leontsinis, S.; Maltezos, S.; Mann, A; Ntekas, K.; Panagiotopoulou, E. St.; Papadopoulou, Th. D.; Tsipolitis, G.; Vlachos, S.] Tomsk State Univ, Tomsk, Russia.
[Andeen, T.; Conventi, F.; Della Pietra, M.; Ilchenko, Y.; Narayan, R.; Onyisi, P. U. E.] Univ Napoli Parthenope, Naples, Italy.
[Abdinov, O.; Corriveau, F.; Khalil-Zada, F.; McPherson, R. A.; Robertson, S. H.; Sobie, R.; Teuscher, R. J.] Inst Particle Phys IPP, Ottawa, ON, Canada.
[Bosman, M.; Casolino, M.; Cavallaro, E.; Cavalli-Sforza, M.; Cortes-Gonzalez, A.; Fischer, C.; Gerbaudo, D.; Parra, G. Gonzalez; Rozas, A. Juste; Korolkov, I.; Lange, J. C.; Paz, I. Lopez; Martinez, M.; Mir, L. M.; Pages, A. Pacheco; Aranda, C. Padilla; Riu, I.; Rizzi, C.; Perez, A. Rodriguez; Valery, L.] Natl Inst Phys & Nucl Engn, Bucharest, Romania.
[Abulaiti, Y.; Agatonovic-Jovin, T.; Bogavac, D.; Bokan, P.; Campoverde, A.; Dimitrievska, A.; Fedin, O. L.; Krstic, J.; Marjanovic, M.; Popovic, D. S.; Sijacki, Dj.; Simic, Lj.; Vranjes, N.; Milosavljevic, M. Vranjes; Zivkovic, L.] St Petersburg State Polytech Univ, Dept Phys, St Petersburg, Russia.
[Buanes, T.; Dale, O.; Eigen, G.; Geng, C.; Guo, Y.; Kastanas, A.; Li, B.; Liebig, W.; Lipniacka, A.; Maeland, S.; Latour, B. Martin Dit; Smestad, L.; Stugu, B.; Yang, Z.; Zalieckas, J.] Univ Michigan, Dept Phys, Ann Arbor, MI 48109 USA.
[Amadio, B. T.; Axen, B.; Barnett, R. M.; Beringer, J.; Bhimji, W.; Brosamer, J.; Calafiura, P.; Cerutti, F.; Ciocio, A.; Clarke, R. N.; Cooke, M.; Duffield, E. M.; Einsweiler, K.; Farrell, S.; Gabrielli, A.; Garcia-Sciveres, M.; Gilchriese, M.; Govender, N.; Haber, C.; Heim, T.; Heinemann, B.; Hinchliffe, I.; Hinman, R. R.; Holmes, T. R.; Jeanty, L.; Leggett, C.; Marshall, Z.; Ohm, C. C.; Griso, S. Pagan; Potamianos, K.; Pranko, A.; Shapiro, M.; Sood, A.; Tibbetts, M. J.; Trottier-McDonald, M.; Tsulaia, V.; Viel, S.; Wang, H.; Yao, W-M.; Yu, D. R.] Ctr High Performance Comp, CSIR Campus, Cape Town, South Africa.
[Biedermann, D.; Dietrich, J.; Giorgi, F. M.; Grancagnolo, S.; Greenwood, Z. D.; Herbert, G. H.; Hristova, I.; Kind, O. M.; Kolanoski, H.; Lacker, H.; Lohse, T.; Mergelmeyer, S.; Nikiforov, A.; Rehnisch, L.; Rieck, P.; Sawyer, L.; Schulz, H.; Sperlich, D.; Stamm, S.; zur Nedden, M.] Louisiana Tech Univ, Ruston, LA 71270 USA.
[Beck, H. P.; Cervelli, A.; Ereditato, A.; Grinstein, S.; Haug, S.; Rozas, A. Juste; Martinez, M.; Meloni, F.; Mullier, G. A.; Rimoldi, M.; Stramaglia, M. E.; Weber, M. S.] ICREA, Barcelona, Spain.
[Bella, L. Aperio; Bracinik, J.; Broughton, J. H.; Casadei, D.; Charlton, D. G.; Chisholm, A. S.; Daniells, A. C.; Foster, A. G.; Gonella, L.; Hanagaki, K.; Hawkes, C. M.; Levy, M.; Quijada, J. A. Murillo; Nikolopoulos, K.; Thomas, J. P.; Watson, A. T.; Wilson, J. A.] Osaka Univ, Grad Sch Sci, Osaka, Japan.
[Arik, M.; Beddall, A. J.; Beddall, A.; Bingul, A.; Cetin, S. A.; Hsu, P. J.; Istin, S.; Ozcan, V. E.] Natl Tsing Hua Univ, Dept Phys, Taipei, Taiwan.
[Igonkina, O.; Losada, M.; Moreno, D.; Navarro, G.; Sandoval, C.] Radboud Univ Nijmegen Nikhef, Inst Math Astrophys & Particle Phys, Nijmegen, Netherlands.
[Alberghi, G. L.; Bellagamba, L.; Biondi, S.; Boscherini, D.; Bruni, A.; Bruni, G.; Bruschi, M.; D'amen, G.; De Castro, S.; Fabbri, F.; Fabbri, L.; Franchini, M.; Gabrielli, A.; Giacobbe, B.; Giorgi, F. M.; Grafstroem, R.; Ilchenko, Y.; Massa, I.; Massa, L.; Mengarelli, A.; Negrini, M.; Onyisi, P. U. E.; Piccinini, M.; Polini, A.; Rinaldi, L.; Romano, M.; Sbarra, C.; Sbrizzi, A.; Semprini-Cesari, N.; Sidoti, A.; Sioli, M.; Spighi, R.; Tupputi, S. A.; Ucchielli, G.; Valentinetti, S.; Villa, M.; Vittori, C.; Zoccoli, A.] Univ Texas Austin, Dept Phys, Austin, TX 78712 USA.
[Arslan, O.; Bechtle, R.; Bernlochner, F. U.; Brock, I.; Bruscino, N.; Cioara, I. A.; Cristinziani, M.; Davey, W.; Desch, K.; Dingfelder, J.; Gaycken, G.; Geich-Gimbel, Ch.; Ghneimat, M.; Grefe, C.; Haefner, R.; Hageboeck, S.; Hansen, M. C.; Hohn, D.; Huegging, F.; Janssen, J.; Jenni, P.; Kostyukhin, V. V.; Kraus, J. K.; Kroseberg, J.; Krueger, H.; Lantzsch, K.; Lassnig, M.; Lenz, T.; Leyko, A. M.; Liebal, J.; Mann, A; Mijovic, L.; Moles-Valls, R.; Obermann, T.; Pohl, D.; Ricken, O.; Sarrazin, B.; Schaepe, S.; Schopf, E.; Schultens, M. J.; Schwindt, T.; Seema, P.; Stillings, J. A.; von Toerne, E.; Wagner, P.; Wang, T.; Wermes, N.; Wienemann, P.; Wiik-Fuchs, L. A. M.; Winter, B. T.; Wong, K. H. Yau; Yuen, S. P. Y.; Zhang, R.] CERN, Geneva, Switzerland.
[Ahlen, S. P.; Black, K. M.; Butler, J. M.; Dell'Asta, L.; Helary, L.; Khubua, J.; Kruskal, M.; Long, B. A.; Shank, J. T.; Yan, Z.; Youssef, S.] Georgian Tech Univ GTU, Tbilisi, Rep of Georgia.
[Amelung, C.; Amundsen, G.; Barone, G.; Bensinger, J. R.; Bianchini, L.; Blocker, C.; Coffey, L.; Dhaliwal, S.; Kono, T.; Loew, K. M.; Nagai, R.; Sciolla, G.; Venturini, A.; Zengel, K.] Ochanomizu Univ, Ochadai Acad Prod, Tokyo, Japan.
[Coutinho, Y. Amaral; Caloba, L. P.; Cerqueira, A. S.; do Vale, M. A. B.; Donadelli, M.; Konoplich, R.; Navarro, J. L. La Rosa; Leite, M. A. L.; Maidantchik, C.; de Andrade Filho, L. Manhaes; Marroquim, F.; Nepomuceno, A. A.; Peralva, B. S.; Seixas, J. M.] Manhattan Coll, New York, NY USA.
[Adams, D. L.; Assamagan, K.; Begel, M.; Buttinger, W.; Chen, H.; Chernyatin, V.; Debbe, R.; Elmsheuser, J.; Ernst, M.; Gibbard, B.; Gordon, H. A.; Lakovidis, G.; Klimentov, A.; Kouskoura, V.; Kravchenko, A.; Lanni, F.; Manghi, F. Lasagni; Lee, C. A.; Leisos, A.; Liu, H.; Lynn, D.; Ma, H.; Maeno, T.; Mann, A; Mountricha, E.; Nevski, P.; Nilsson, P.; Damazio, D. Oliveira; Paige, F.; Panitkin, S.; Perepelitsa, D. V.; Pleier, M. -A.; Polychronakos, V.; Protopopescu, S.; Purohit, M.; Radeka, V.; Rajagopalan, S.; Redlinger, G.; Snyder, S.; Steinberg, P.; Takai, H.; Tricoli, A.; Undrus, A.; Wenaus, T.; Xu, L.; Ye, S.] Hellen Open Univ, Patras, Greece.
[Lin, S. C.] Acad Sinica, Acad Sinica Grid Comp, Inst Phys, Taipei, Taiwan.
[Sola, J. D. Bossio; Liu, B.; Marceca, G.; Otero y Garzon, G.; Piegaia, R.; Reisin, H.; Sacerdoti, S.] Shandong Univ, Sch Phys, Shandong, Peoples R China.
[Brochu, F. M.; Brunt, B. H.; Lester, C. G.; Myagkov, A. G.; Potter, C. J.; Robinson, D.; Ward, C. P.; Zaitsev, A. M.] State Univ, Moscow Inst Phys & Technol, Dolgoprudnyi, Russia.
[Bellerive, A.; Cree, G.; Di Valentino, D.; Gillberg, D.; Koffas, T.; Lacey, J.; Leight, W. A.; Mann, A; Nessi, M.; Nomidis, I.; Oakham, F. G.; Pasztor, G.; Ruiz-Martinez, A.; Vincter, M. G.] Univ Geneva, Sect Phys, Geneva, Switzerland.
[Aleksa, M.; Aloisio, A.; Alonso, A.; Gonzalez, B. Alvarez; Amorim, A.; Amoroso, S.; Anders, G.; Andreazza, A.; Angerami, A.; Anghinolfi, F.; Annovi, A.; Antonov, A.; Arnaez, O.; Avolio, G.; Baak, M. A.; Backes, M.; Backhaus, M.; Barak, L.; Beermann, T. A.; Beltramello, O.; Bianco, M.; Bogaerts, J. A.; Bortfeldt, J.; Boveia, A.; Boyd, J.; Burckhart, H.; Camarda, S.; Campana, S.; Garrido, M. D. M. Capeans; Carli, T.; Carrillo-Montoya, G. D.; Catinaccio, A.; Cattai, A.; Cerv, M.; Chromek-Burckhart, D.; Colombo, T.; Conti, G.; Dell'Acqua, A.; Deviveiros, P. O.; Di Girolamo, A.; Di Girolamo, B.; Di Nardo, R.; Dittus, F.; Dobos, D.; Dudarev, A.; Duehrssen, M.; Eifert, T.; Ellis, N.; Elsing, M.; Faltova, J.; Farthouat, R.; Fassnacht, P.; Feng, E. J.; Francis, D.; Fressard-Batraneanu, S. M.; Froidevaux, D.; Gadatsch, S.; Goossens, L.; Gorini, B.; Gray, H. M.; Gumpert, C.; Hawkings, R. J.; Helsens, C.; Correia, A. M. Henriques; Hervas, L.; Huhtinen, M.; Iengo, P.; Jakobsen, S.; Klioutchnikova, T.; Krasznahorkay, A.; Lapoire, C.; Law, A. T.; Miotto, G. Lehmann; Lenzi, B.; Lichard, P.; Malyukov, S.; Mandelli, B.; Mann, A; Mapelli, L.; Marzin, A.; Berlingen, J. Montejo; Mornacchi, G.; Nairz, A. M.; Nakahama, Y.; Nessi, M.; Nordberg, M.; Oide, H.; Palestini, S.; Pasztor, G.; Pauly, T.; Pernegger, H.; Petersen, B. A.; Pommes, K.; Poppleton, A.; Poulard, G.; Poveda, J.; Astigarraga, M. E. Pozo; Rammensee, M.; Raymond, M.; Rembser, C.; Ritsch, E.; Roe, S.; Ruthmann, N.; Salzburger, A.; Schaefer, D.; Schlenker, S.; Schmieden, K.; Sforza, F.; Sanchez, C. A. Solans; Spigu, G.; Starz, S.; Stelzer, H. J.; Teischinger, F. A.; Ten Kate, H.; Unal, G.; van Woerden, M. C.; Vandelli, W.; Voss, R.; Vuillermet, R.; Wells, P. S.; Wengler, T.; Wenig, S.; Werner, P.; Wilkens, H. G.; Wotschack, J.; Young, C. J. S.; Zwalinski, L.] Eotvos Lorand Univ, Budapest, Hungary.
[Alison, J.; Anderson, K. J.; Bryant, P.; Toro, R. Camacho; Cheng, Y.; Dandoy, J. R.; Facini, G.; Gardner, R. W.; Kapliy, A.; Kim, Y. K.; Krizka, K.; Li, H. L.; Mann, A; Merritt, F. S.; Miller, D. W.; Okumura, Y.; Oreglia, M. J.; Piacquadio, G.; Pilcher, J. E.; Saxon, J.; Shochet, M. J.; Stark, G. H.; Swiatlowski, M.; Vukotic, I.; Wu, M.] SUNY Stony Brook, Dept Phys & Astron, Stony Brook, NY 11794 USA.
[Alison, J.; Anderson, K. J.; Bryant, P.; Toro, R. Camacho; Cheng, Y.; Dandoy, J. R.; Facini, G.; Gardner, R. W.; Kapliy, A.; Kim, Y. K.; Krizka, K.; Li, H. L.; Merritt, F. S.; Miller, D. W.; Okumura, Y.; Oreglia, M. J.; Piacquadio, G.; Pilcher, J. E.; Saxon, J.; Shochet, M. J.; Stark, G. H.; Swiatlowski, M.; Vukotic, I.; Wu, M.] SUNY Stony Brook, Dept Chem, Stony Brook, NY 11794 USA.
[Pinamonti, M.] Int Sch Adv Studies SISSA, Trieste, Italy.
[Purohit, M.] Univ S Carolina, Dept Phys & Astron, Columbia, SC 29208 USA.
[Boumediene, D.; Busato, E.; Calvet, D.; Calvet, S.; Chomont, A. R.; Donini, J. .; Gris, Ph.; Madar, R.; Pallin, D.; Saez, S. M. Romano; Santoni, C.; Shi, L.; Simon, D.; Vazeille, F.] Sun Yat Sen Univ, Sch Phys & Engn, Guangzhou, Guangdong, Peoples R China.
[Alkire, S. P.; Angerami, A.; Brooijmans, G.; Carbone, R. M.; Clark, M. R.; Cole, B.; Hu, D.; Hughes, E. W.; Iordanidou, K.; Klein, M. H.; Mohapatra, S.; Ochoa, I.; Parsons, J. A.; Shiyakova, M.; Smith, M. N. K.; Smith, R. W.; Thompson, E. N.; Tuts, P. M.; Wang, T.; Zhou, L.] Bulgarian Acad Sci, Inst Nucl Res & Nucl Energy INRNE, Sofia, Bulgaria.
[Alonso, A.; Besjes, G. J.; Dam, M.; Galster, G.; Hansen, J. B.; Hansen, J. D.; Hansen, P. H.; Loevschall-Jensen, A. E.; Monk, J.; Mortensen, S. S.; Pedersen, L. E.; Petersen, T. C.; Pinge, A.; Smirnova, L. N.; Turchikhin, S.; Wiglesworth, C.; Xella, S.] Moscow MV Lomonosov State Univ, Fac Phys, Moscow, Russia.
[Song, H. Y.; Zhang, G.] Acad Sinica, Inst Phys, Taipei, Taiwan.
[Tikhomirov, V. O.] Natl Res Nucl Univ MEPhI, Moscow, Russia.
[Banas, E.; de Renstrom, P. A. Bruckman; Burka, K.; Chwastowski, J. J.; Derendarz, D.; Godlewski, J.; Gornicki, E.; Kaczmarska, A.; Knapik, J. .; Korcyl, K.; Kowalewska, A. B.; Malecki, Pa.; Olszewski, A.; Olszowska, J.; Stanecka, E.; Staszewski, R.; Tompkins, L.; Trzebinski, M.; Trzupek, A.; Wolter, M. W.; Wosiek, B. K.; Wozniak, K. W.; Zabinski, B.] Stanford Univ, Dept Phys, Stanford, CA 94305 USA.
[Cao, T.; Firan, A.; Hetherly, J. W.; Kama, S.; Kehoe, R.; Sekula, S. J.; Stroynowski, R.; Toth, J.; Turvey, A. J.; Varol, T.; Wang, H.; Ye, J.; Zhao, X.; Zhou, L.] Wigner Res Ctr Phys, Inst Particle & Nucl Phys, Budapest, Hungary.
[Izen, J. M.; Leyton, M.; Meirose, B.; Namasivayam, H.; Reeves, K.; Vest, A.] Flensburg Univ Appl Sci, Flensburg, Germany.
[Asbah, N.; Behr, J. K.; Bertsche, C.; Bessner, M.; Bloch, I.; Britzger, D.; Deterre, C.; Dutta, B.; Dyndal, M.; Eckardt, C.; Filipuzzi, M.; Flaschel, N.; Bravo, A. Gascon; Gregor, I. M.; Haleem, M.; Hamnett, P. G.; Hiller, K. H.; Howarth, J.; Huang, Y.; Katzy, J.; Keller, J. S.; Kondrashova, N.; Kuh, T.; Lobodzinska, E.; Lohwasser, K.; Madsen, A.; Medinnis, M.; Moenig, K.; Garcia, R. F. Naranjo; Naumann, T.; O'Rourke, A. A.; Peschke, R.; Peters, K.; Pirumov, H.; Poley, A.; Robinson, J. E. M.; Schaefer, R.; Schmitt, S.; South, D.; Stanescu-Bellu, M.; Stanitzki, M. M.; Styles, N. A.; Tackmann, K.; Trofymov, A.; Wang, J.; Yusuff, I.; Zakharchuk, N.] Univ Malaya, Dept Phys, Kuala Lumpur, Malaysia.
[Burmeister, I.; Cinca, D.; Dette, K.; Erdmann, J.; Esch, H.; Gonella, G.; Goessling, C.; Grohs, J. P.; Homann, M.; Jentzsch, J.; Klingenberg, R.; Kroeninger, K.; Zhang, R.] Aix Marseille Univ, CPPM, Marseille, France.
[Burmeister, I.; Cinca, D.; Dette, K.; Erdmann, J.; Esch, H.; Gonella, G.; Goessling, C.; Grohs, J. P.; Homann, M.; Jentzsch, J.; Klingenberg, R.; Kroeninger, K.; Zhang, R.] CNRS IN2P3, Marseille, France.
[Anger, R.; Duschinger, D.; Friedrich, F.; Gutschow, C.; Hauswald, L.; Kobel, M.; Mader, W. F.; Novgorodova, O.; Siegert, F.; Socher, F.; Straessner, A.; Vest, A.; Wahrmund, S.] PKU CHEP, Beijing, Peoples R China.
RI Kuday, Sinan/C-8528-2014; Doyle, Anthony/C-5889-2009; Mitsou,
Vasiliki/D-1967-2009; Solodkov, Alexander/B-8623-2017; Camarri,
Paolo/M-7979-2015; Carvalho, Joao/M-4060-2013; Prokoshin,
Fedor/E-2795-2012; Guo, Jun/O-5202-2015; Livan, Michele/D-7531-2012;
Gladilin, Leonid/B-5226-2011; Villa, Mauro/C-9883-2009; Peleganchuk,
Sergey/J-6722-2014; messina, andrea/C-2753-2013; Yang,
Haijun/O-1055-2015; White, Ryan/E-2979-2015; Li, Liang/O-1107-2015;
Monzani, Simone/D-6328-2017; Warburton, Andreas/N-8028-2013; Tikhomirov,
Vladimir/M-6194-2015
OI Kuday, Sinan/0000-0002-0116-5494; Doyle, Anthony/0000-0001-6322-6195;
Mitsou, Vasiliki/0000-0002-1533-8886; Solodkov,
Alexander/0000-0002-2737-8674; Camarri, Paolo/0000-0002-5732-5645;
Carvalho, Joao/0000-0002-3015-7821; Prokoshin,
Fedor/0000-0001-6389-5399; Guo, Jun/0000-0001-8125-9433; Livan,
Michele/0000-0002-5877-0062; Gladilin, Leonid/0000-0001-9422-8636;
Villa, Mauro/0000-0002-9181-8048; Peleganchuk,
Sergey/0000-0003-0907-7592; White, Ryan/0000-0003-3589-5900; Li,
Liang/0000-0001-6411-6107; Monzani, Simone/0000-0002-0479-2207;
Warburton, Andreas/0000-0002-2298-7315; Tikhomirov,
Vladimir/0000-0002-9634-0581
FU ANPCyT, Argentina; YerPhI, Armenia; ARC, Australia; BMWFW, Austria; FWF,
Austria; ANAS, Azerbaijan; SSTC, Belarus; CNPq, Brazil; FAPESP, Brazil;
NSERC, Canada; NRC, Canada; CFI, Canada; CERN; CONICYT, Chile; CAS,
China; MOST, China; NSFC, China; COLCIENCIAS, Colombia; MSMT CR, Czech
Republic; MPO CR, Czech Republic; VSC CR, Czech Republic; DNRF, Denmark;
DNSRC, Denmark; IN2P3-CNRS, CEA-DSM/IRFU, France; GNSF, Georgia; BMBF,
Germany; HGF, Germany; MPG, Germany; GSRT, Greece; RGC, Hong Kong SAR,
China; ISF, Israel; I-CORE, Israel; Benoziyo Center, Israel; INFN,
Italy; MEXT, Japan; JSPS, Japan; CNRST, Morocco; FOM, Netherlands; NWO,
Netherlands; RCN, Norway; MNiSW, Poland; NCN, Poland; FCT, Portugal;
MNE/IFA, Romania; MES of Russia, Russian Federation; NRC KI, Russian
Federation; JINR; MESTD, Serbia; MSSR, Slovakia; ARRS, Slovenia; MIZS,
Slovenia; DST/NRF, South Africa; MINECO, Spain; SRC, Sweden; Wallenberg
Foundation, Sweden; SERI, Switzerland; SNSF, Switzerland; Canton of
Bern, Switzerland; Cantons of Geneva, Switzerland; MOST, Taiwan; TAEK,
Turkey; STFC, United Kingdom; DOE, United States of America; NSF, United
States of America; BCKDF, Canada; Canada Council, Canada; Canarie,
Canada; CRC, Canada; Compute Canada, Canada; FQRNT, Canada; Ontario
Innovation Trust, Canada; EPLANET, European Union; ERC, European Union;
FP7, European Union; Horizon, European Union; Marie Sklodowska-Curie
Actions, European Union; Investissement d'Avenir Labex, France;
Investissement d'Avenir Idex, France; ANR, France; Region Auvergne,
France; Fondation Partager le Savoir, France; DFG, Germany; AvH
Foundation, Germany; Herakleitos programme; Thales programme; Aristeia
programme - EU-ESF; Greek NSRF; BSF, Israel; GIF, Israel; Minerva,
Israel; BRF, Norway; Generalitat de Catalunya, Generalitat Valenciana,
Spain; Royal Society, United Kingdom; Leverhulme Trust, United Kingdom
FX We acknowledge the support of ANPCyT, Argentina; YerPhI, Armenia; ARC,
Australia; BMWFW and FWF, Austria; ANAS, Azerbaijan; SSTC, Belarus; CNPq
and FAPESP, Brazil; NSERC, NRC and CFI, Canada; CERN; CONICYT, Chile;
CAS, MOST and NSFC, China; COLCIENCIAS, Colombia; MSMT CR, MPO CR and
VSC CR, Czech Republic; DNRF and DNSRC, Denmark; IN2P3-CNRS,
CEA-DSM/IRFU, France; GNSF, Georgia; BMBF, HGF, and MPG, Germany; GSRT,
Greece; RGC, Hong Kong SAR, China; ISF, I-CORE and Benoziyo Center,
Israel; INFN, Italy; MEXT and JSPS, Japan; CNRST, Morocco; FOM and NWO,
Netherlands; RCN, Norway; MNiSW and NCN, Poland; FCT, Portugal; MNE/IFA,
Romania; MES of Russia and NRC KI, Russian Federation; JINR; MESTD,
Serbia; MSSR, Slovakia; ARRS and MIZS, Slovenia; DST/NRF, South Africa;
MINECO, Spain; SRC and Wallenberg Foundation, Sweden; SERI, SNSF and
Cantons of Bern and Geneva, Switzerland; MOST, Taiwan; TAEK, Turkey;
STFC, United Kingdom; DOE and NSF, United States of America. In
addition, individual groups and members have received support from
BCKDF, the Canada Council, Canarie, CRC, Compute Canada, FQRNT, and the
Ontario Innovation Trust, Canada; EPLANET, ERC, FP7, Horizon 2020 and
Marie Sklodowska-Curie Actions, European Union; Investissements d'Avenir
Labex and Idex, ANR, Region Auvergne and Fondation Partager le Savoir,
France; DFG and AvH Foundation, Germany; Herakleitos, Thales and
Aristeia programmes co-financed by EU-ESF and the Greek NSRF; BSF, GIF
and Minerva, Israel; BRF, Norway; Generalitat de Catalunya, Generalitat
Valenciana, Spain; the Royal Society and Leverhulme Trust, United
Kingdom.
NR 57
TC 1
Z9 1
U1 24
U2 24
PU ELSEVIER SCIENCE BV
PI AMSTERDAM
PA PO BOX 211, 1000 AE AMSTERDAM, NETHERLANDS
SN 0370-2693
EI 1873-2445
J9 PHYS LETT B
JI Phys. Lett. B
PD OCT 10
PY 2016
VL 761
BP 136
EP 157
DI 10.1016/j.physletb.2016.08.019
PG 22
WC Astronomy & Astrophysics; Physics, Nuclear; Physics, Particles & Fields
SC Astronomy & Astrophysics; Physics
GA DX6CI
UT WOS:000384469900023
ER
PT J
AU Aaboud, M
Aad, G
Abbott, B
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CA ATLAS Collaboration
TI Measurement of the total cross section from elastic scattering in pp
collisions at root s=8 TeV with the ATLAS detector
SO PHYSICS LETTERS B
LA English
DT Article
ID HIGH-ENERGY; LHC ENERGY; INTERFERENCE; MODEL
AB A measurement of the total ppcross section at the LHC at root s = 8TeV is presented. An integrated luminosity of 500 mu b(-1) was accumulated in a special run with high-beta* beam optics to measure the differential elastic cross section as a function of the Mandelstam momentum transfer variable t. The measurement is performed with the ALFA sub-detector of ATLAS. Using a fit to the differential elastic cross section in the -t range from 0.014 GeV2 to 0.1 GeV2 to extrapolate t -> 0, the total cross section, sigma(tot)( pp -> X), is measured via the optical theorem to be
sigma(tot)(pp -> X) = 96.07 +/- 0.18 (stat.) +/- 0.85 (exp.) +/- 0.31 (extr.) mb,
where the first error is statistical, the second accounts for all experimental systematic uncertainties and the last is related to uncertainties in the extrapolation t -> 0. In addition, the slope of the exponential function describing the elastic cross section at small t is determined to be B = 19.74 +/- 0.05 (stat.) +/- 0.23 (syst.) GeV-2. (C) 2016 The Author. Published by Elsevier B.V.
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[Cakira, O.; Ciftci, A. K.; Yildiz, H. Duran] Ankara Univ, Dept Phys, Ankara, Turkey.
[Kuday, S.] Istanbul Aydin Univ, Istanbul, Turkey.
[Sultansoy, S.] TOBB Univ Econ & Technol, Div Phys, Ankara, Turkey.
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[Barnovska-Blenessy, Z.; Berger, N.; Delmastro, M.; Di Ciaccio, L.; Elles, S.; Grevtsov, K.; Guillemin, T.; Hryn'ova, T.; Jezequel, S.; Koletsou, I.; Lafaye, R.; Leveque, J.; Mastrandrea, P.; Sauvan, E.; Smart, B. H.; Todorov, T.; Wingerter-Seez, I.; Yatsenko, E.] Univ Savoie Mt Blanc, Annecy Le Vieux, France.
[Blair, R. E.; Chekanov, S.; LeCompte, T.; Love, J.; Malon, D.; Metcalfe, J.; Nguyen, D. H.; Paramonov, A.; Price, L. E.; Proudfoot, J.; Ryu, S.; Stanek, R. W.; van Gemmeren, P.; Wang, R.; Webster, J. S.; Yoshida, R.; Zhang, J.] Argonne Natl Lab, Div High Energy Phys, Argonne, IL 60439 USA.
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[Brandt, A.; Bullock, D.; Darmora, S.; De, K.; Farbin, A.; Feremenga, L.; Griffiths, J.; Hadavand, H. K.; Heelan, L.; Kim, H. Y.; Ozturk, N.; Schovancova, J.; Stradling, A. R.; Usai, G.; Vartapetian, A.; Warburton, A.; White, A.; Yu, J.] Univ Texas Arlington, Dept Phys, POB 19059, Arlington, TX 76019 USA.
[Angelidakis, S.; Chouridou, S.; Fassouliotis, D.; Giokaris, N.; Ioannou, P.; Kourkoumelis, C.; Tsirintanis, N.] Univ Athens, Dept Phys, Athens, Greece.
[Alexopoulos, T.; Benekos, N.; Dris, M.; Gazis, E. N.; Karakostas, K.; Karastathis, N.; Karentzos, E.; Leontsinis, S.; Maltezos, S.; Panagiotopoulou, E. St.; Papadopoulou, Th. D.; Tsipolitis, G.; Vlachos, S.] Natl Tech Univ Athens, Dept Phys, Zografos, Greece.
[Andeen, T.; Ilchenko, Y.; Narayan, R.; Onyisi, P. U. E.] Univ Texas Austin, Dept Phys, Austin, TX 78712 USA.
[Abdinov, O.; Khalil-zada, F.] Azerbaijan Acad Sci, Inst Phys, Baku, Azerbaijan.
[Anjos, N.; Bosman, M.; Casado, M. P.; Casolino, M.; Cavallaro, E.; Cavalli-Sforza, M.; Farooque, T.; Perez, S. Fernandez; Fischer, C.; Fracchia, S.; Gerbaudo, D.; Parra, G. Gonzalez; Grinstein, S.; Rozas, A. Juste; Korolkov, I.; Lange, J. C.; Paz, I. Lopez; Martinez, M.; Mir, L. M.; Pages, A. Pacheco; Aranda, C. Padilla; Riu, I.; Rizzi, C.; Perez, A. Rodriguez; Sorin, V.; Terzo, S.; Tripiana, M. F.; Tsiskaridze, S.; Valery, L.] Barcelona Inst Sci & Technol, Inst Fis Altes Energies IFAE, Barcelona, Spain.
[Agatonovic-Jovin, T.; Bogavac, D.; Bokan, R.; Dimitrievska, A.; Krstic, J.; Marjanovic, M.; Sijacki, Dj.; Simic, Lj.; Vranjes, N.; Milosavljevic, M. Vranjes; Zivkovic, L.] Univ Belgrade, Inst Phys, Belgrade, Serbia.
[Buanes, T.; Dale, O.; Eigen, G.; Kastanas, A.; Liebig, W.; Lipniacka, A.; Maeland, S.; dit Latour, B. Martin; Smestad, L.; Stugu, B.; Yang, Z.; Zalieckas, J.] Univ Bergen, Dept Phys & Technol, Bergen, Norway.
[Amadio, B. T.; Axen, B.; Barnett, R. M.; Beringer, J.; Biebel, O.; Brosamer, J.; Calafiura, P.; Alberich, L. Cerda; Cerutti, F.; Ciocio, A.; Clarke, R. N.; Cooke, M.; Duffield, E. M.; Einsweiler, K.; Farrell, S.; Firan, A.; Gabrielli, A.; Garcia-Sciveres, M.; Gilchriese, M.; Haber, C.; Heim, T.; Heinemann, B.; Hinchliffe, I.; Hinman, R. R.; Holmes, T. R.; Jeanty, L.; Lavrijsen, W.; Leggett, C.; Marshall, Z.; Ohm, C. C.; Griso, S. Pagan; Potamianos, K.; Pranko, A.; Shapiro, M.; Sood, A.; Spangenberg, M.; Tibbetts, M. J.; Trottier-McDonald, M.; Tsulaia, V.; Viel, S.; Wang, H.; Yao, W-M.; Yu, D. R.] Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Div Phys, Berkeley, CA 94720 USA.
[Aloisio, A.; Amadio, B. T.; Axen, B.; Barnett, R. M.; Beringer, J.; Biebel, O.; Brosamer, J.; Calafiura, P.; Alberich, L. Cerda; Cerutti, F.; Ciocio, A.; Clarke, R. N.; Cooke, M.; Duffield, E. M.; Einsweiler, K.; Farrell, S.; Firan, A.; Gabrielli, A.; Garcia-Sciveres, M.; Gilchriese, M.; Haber, C.; Heim, T.; Heinemann, B.; Hinchliffe, I.; Hinman, R. R.; Holmes, T. R.; Jeanty, L.; Lavrijsen, W.; Leggett, C.; Maio, A.; Marshall, Z.; Ohm, C. C.; Griso, S. Pagan; Potamianos, K.; Pranko, A.; Shapiro, M.; Sood, A.; Spangenberg, M.; Tibbetts, M. J.; Trottier-McDonald, M.; Tsulaia, V.; Viel, S.; Wang, H.; Yao, W-M.; Yu, D. R.] Univ Calif Berkeley, Berkeley, CA 94720 USA.
[Biedermann, D.; Dietrich, J.; Giorgi, F. M.; Grancagnolo, S.; Herbert, G. H.; Hristova, I.; Kind, O. M.; Kolanoski, H.; Lacker, H.; Lohse, T.; Mergelmeyer, S.; Nikiforov, A.; Rehnisch, L.; Rieck, P.; Schulz, H.; Sperlich, D.; Stamm, S.; zur Nedden, M.] Humboldt Univ, Dept Phys, Berlin, Germany.
[Beck, H. P.; Cervelli, A.; Ereditato, A.; Haug, S.; Meloni, F.; Miucci, A.; Mullier, G. A.; Rimoldi, M.; Stramaglia, M. E.; Weber, M. S.] Univ Bern, Albert Einstein Ctr Fundamental Phys, Bern, Switzerland.
[Beck, H. P.; Cervelli, A.; Ereditato, A.; Haug, S.; Meloni, F.; Miucci, A.; Mullier, G. A.; Rimoldi, M.; Stramaglia, M. E.; Weber, M. S.] Univ Bern, High Energy Phys Lab, Bern, Switzerland.
[Allport, P. P.; Andari, N.; Bella, L. Aperio; Baca, M. J.; Bracinik, J.; Broughton, J. H.; Casadei, D.; Charlton, D. G.; Daniells, A. C.; Foster, A. G.; Gonella, L.; Hawkes, C. M.; Head, S. J.; Hillier, S. J.; Levy, M.; Mudd, R. D.; Quijada, J. A. Murillo; Newman, P. R.; Nikolopoulos, K.; Owen, R. E.; Slater, M.; Thomas, J. P.; Thompson, P. D.; Watkins, P. M.; Watson, A. T.; Watson, M. F.; Wilson, J. A.] Univ Birmingham, Sch Phys & Astron, Birmingham, W Midlands, England.
[Arik, M.; Ozcan, V. E.] Bogazici Univ, Dept Phys, Istanbul, Turkey.
[Beddall, A.; Bingul, A.] Gaziantep Univ, Dept Engn Phys, Gaziantep, Turkey.
[Cetin, S. A.] Istanbul Bilgi Univ, Fac Engn & Nat Sci, Istanbul, Turkey.
[Beddall, A. J.] Bahcesehir Univ, Fac Engn & Nat Sci, Istanbul, Turkey.
[Losada, M.; Moreno, D.; Navarro, G.; Sandoval, C.] Univ Antonio Narino, Ctr Invest, Bogota, Colombia.
[Arik, M.; Ozcan, V. E.] Univ Bologna, Sez Bologna, Ist Nazl Fis Nucl, Bologna, Italy.
[Alberghi, G. L.; Biondi, S.; Cabras, G.; Ciocca, C.; D'amen, G.; De Castro, S.; Fabbri, F.; Fabbri, L.; Franchini, M.; Gabrielli, A.; Grafstrom, P.; Magnhi, F. Lasagni; Massa, I.; Massa, L.; Mengarelli, A.; Piccinini, M.; Romano, M.; Sbrizzi, A.; Semprini-Cesari, N.; Sidoti, A.; Sioli, M.; Tupputi, S. A.; Ucchielli, G.; Valentinetti, S.; Villa, M.; Vittori, C.; Zoccoli, A.] Univ Bologna, Dipartimento Fis & Astron, Bologna, Italy.
[Arslan, O.; Bechtle, R.; Bernlochner, F. U.; Brock, I.; Bruscino, N.; Caudron, J.; Cioara, I. A.; Cristinziani, M.; Davey, W.; Desch, K.; Dingfelder, J.; Gaycken, G.; Geich-Gimbel, Ch.; Ghneimat, M.; Grefe, C.; Hageboeck, S.; Hansen, M. C.; Hohn, D.; Huegging, F.; Janssen, J.; Kostyukhin, V. V.; Kroseberg, J.; Krueger, H.; Lantzsch, K.; Lenz, T.; Leyko, A. M.; Liebal, J.; Moles-Valls, R.; Obermann, T.; Ricken, O.; Sarrazin, B.; Schaepe, S.; Schopf, E.; Schultens, M. J.; Schwindt, T.; Seema, P.; Stillings, J. A.; von Toerne, E.; Wagner, P.; Wang, T.; Wermes, N.; Wiik-Fuchs, L. A. M.; Winter, B. T.; Wong, K. H. Yau; Yuen, S. P. Y.; Zhang, R.] Univ Bonn, Inst Phys, Bonn, Germany.
[Ahlen, S. P.; Butler, J. M.; Dell'Asta, L.; Kruskal, M.; Long, B. A.; Shank, J. T.; Yan, Z.; Youssef, S.] Boston Univ, Dept Phys, 590 Commonwealth Ave, Boston, MA 02215 USA.
[Amelung, C.; Amundsen, G.; Barone, G.; Bensinger, J. R.; Bianchini, L.; Blocker, C.; Dhaliwal, S.; Goblirsch-Kolb, M.; Herde, H.; Loew, K. M.; Sciolla, G.; Venturini, A.; Zengel, K.] Brandeis Univ, Dept Phys, Waltham, MA 02254 USA.
[Coutinho, Y. Amaral; Caloba, L. P.; Maidantchik, C.; Marroquim, F.; Nepomuceno, A. A.; Seixas, J. M.] Univ Fed Rio De Janeiro COPPE EE IF, Rio De Janeiro, Brazil.
[Cerqueira, A. S.; de Andrade Filho, L. Manhaes; Peralva, B. S.] Fed Univ Juiz de Fora UFJF, Elect Circuits Dept, Juiz De Fora, Brazil.
[do Vale, M. A. B.] Fed Univ Sao Joao del Rei UFSJ, Sao Joao Del Rei, Brazil.
[Donadelli, M.; Navarro, J. L. La Rosa; Leite, M. A. L.] Univ Sao Paulo, Inst Fis, Sao Paulo, Brazil.
[Adams, D. L.; Assamagan, K.; Begel, M.; Chen, H.; Chernyatin, V.; Debbe, R.; Elmsheuser, J.; Ernst, M.; Firan, A.; Gibbard, B.; Gordon, H. A.; Iakovidis, G.; Klimentov, A.; Kouskoura, V.; Kravchenko, A.; Lanni, F.; Lee, C. A.; Liu, H.; Lynn, D.; Ma, H.; Maeno, T.; Mountricha, E.; Nevski, R.; Nilsson, P.; Damazio, D. Oliveira; Paige, F.; Panitkin, S.; Perepelitsa, D. V.; Pleier, M. -A.; Pohl, D.; Polychronakos, V.; Protopopescu, S.; Purohit, M.; Rajagopalan, S.; Redlinger, G.; Snyder, S.; Steinberg, P.; Stucci, S. A.; Takai, H.; Tricoli, A.; Undrus, A.; Wenaus, T.; Xu, L.; Ye, S.] Brookhaven Natl Lab, Dept Phys, Upton, NY 11973 USA.
Transilvania Univ Brasov, Brasov, Romania.
[Alexa, C.; Caprini, I.; Caprini, M.; Chitan, A.; Ciubancan, M.; Constantinescu, S.; Dita, P.; Dita, S.; Dobre, M.; Jinaru, A.; Martoiu, V. S.; Maurer, J.; Olariu, A.; Pantea, D.; Rotaru, M.; Stoicea, G.; Tudorache, A.; Tudorache, V.] Natl Inst Phys & Nucl Engn, Bucharest, Romania.
[Popeneciu, G. A.] Natl Inst Res & Dev Isotop & Mol Technol, Dept Phys, Cluj Napoca, Romania.
Univ Politehn Bucuresti, Bucharest, Romania.
[Gravila, P. M.] West Univ Timisoara, Timisoara, Romania.
[Bossio Sola, J. D.; Marceca, G.; Otero y Garzon, G.; Piegaia, R.; Sacerdoti, S.] Univ Buenos Aires, Dept Fis, Buenos Aires, DF, Argentina.
[Arratia, M.; Barlow, N.; Batley, J. R.; Brochu, F. M.; Brunt, Bh; Carter, J. R.; Chapman, J. D.; Cottin, G.; Gillam, T. P. S.; Hill, J. C.; Kaneti, S.; Lester, C. G.; Malone, C.; Mueller, T.; Parker, M. A.; Potter, C. J.; Robinson, D.; Rosten, J. H. N.; Thomson, M.; Ward, C. P.; Yusuff, I.] Univ Cambridge, Cavendish Lab, Cambridge, England.
[Bellerive, A.; Biebel, O.; Cree, G.; Di Valentino, D.; Gillberg, D.; Koffas, T.; Lacey, J.; Leight, W. A.; Nomidis, I.; Oakham, F. G.; Pasztor, G.; Ruiz-Martinez, A.; Vincter, M. G.; Weber, S. A.] Carleton Univ, Dept Phys, Ottawa, ON, Canada.
[Aleksa, M.; Gonzalez, B. Alvarez; Amoroso, S.; Anders, G.; Anghinolfi, F.; Arnaez, O.; Avolio, G.; Baak, M. A.; Backhaus, M.; Barak, L.; Barisits, M-S; Beermann, T. A.; Beltramello, O.; Bianco, M.; Bogaerts, J. A.; Bortfeldt, J.; Boveia, A.; Boyd, J.; Burckhart, H.; Camarda, S.; Campana, S.; Garrido, M. D. M. Capeans; Carli, T.; Carrillo-Montoya, G. D.; Catinaccio, A.; Cattai, A.; Cery, M.; Chisholm, A. S.; Chromek-Burckhart, D.; Conti, G.; Cortes-Gonzalez, A.; Dell'Acqua, A.; Deviveiros, P. O.; Di Girolamo, A.; Di Girolamo, B.; Di Nardo, R.; Dittus, F.; Dobos, D.; Dudarev, A.; Duhrssen, M.; Ellis, N.; Elsing, M.; Faltova, J.; Farthouat, P.; Fassnacht, P.; Feng, E. J.; Francis, D.; Fressard-Batraneanu, S. M.; Froidevaux, D.; Gadatsch, S.; Goossens, L.; Gorini, B.; Gray, H. M.; Gumpert, C.; Hawkings, R. J.; Helary, L.; Helsens, C.; Correia, A. M. Henriques; Hervas, L.; Hoecker, A.; Huhtinen, M.; Iengo, P.; Jakobsen, S.; Klioutchnikova, T.; Krasznahorkay, A.; Lapoire, C.; Lassnig, M.; Miotto, G. Lehmann; Lenzi, B.; Lichard, P.; Malyukov, S.; Manousos, A.; Mapelli, L.; Marzin, A.; Berlingen, J. Montejo; Morgenstern, S.; Mornacchi, G.; Nairz, A. M.; Nessi, M.; Nordberg, M.; Oide, H.; Palestini, S.; Pauly, T.; Pernegger, H.; Petersen, B. A.; Pommes, K.; Poppleton, A.; Poulard, G.; Poveda, J.; Astigarraga, M. E. Pozo; Rammensee, M.; Raymond, M.; Rembser, C.; Ritsch, E.; Roe, S.; Ruthmann, N.; Salzburger, A.; Schaefer, D.; Schlenker, S.; Schmieden, K.; Sforza, F.; Sanchez, C. A. Solans; Spigo, G.; Starz, S.; Stelzer, H. J.; Teischinger, F. A.; Ten Kate, H.; van Woerden, M. C.; Vandelli, W.; Voss, R.; Vuillermet, R.; Wells, P. S.; Wengler, T.; Wenig, S.; Werner, P.; Wilkens, H. G.; Wotschack, J.; Young, C. J. S.; Zwalinski, L.] CERN, Geneva, Switzerland.
[Alison, J.; Anderson, K. J.; Bryant, R.; Toro, R. Camacho; Cheng, Y.; Dandoy, J. R.; Facini, G.; Gardner, R. W.; Kapliy, A.; Kim, Y. K.; Krizka, K.; Li, H. L.; Merritt, F. S.; Miller, D. W.; Oreglia, M. J.; Pilcher, J. E.; Saxon, J.; Shochet, M. J.; Stark, G. H.; Swiatlowski, M.; Vukotic, I.; Wu, M.] Univ Chicago, Enrico Fermi Inst, 5640 S Ellis Ave, Chicago, IL 60637 USA.
[Blunier, S.; Diaz, M. A.; Ochoa-Ricoux, J. P.] Pontificia Univ Catolica Chile, Dept Fis, Santiago, Chile.
[Brooks, W. K.; Carquin, E.; Kuleshov, S.; Lopez, J. A.; Pezoa, R.; Prokoshin, F.; Loyola, J. E. Salazar; Araya, S. Tapia; Vasquez, G. A.; White, R.] Univ Tecn Federico Santa Maria, Dept Fis, Valparaiso, Chile.
[Bai, Y.; Da Costa, J. Barreiro Guimaraes; Cheng, H. J.; Fang, Y.; Jin, S.; Li, Q.; Liang, Z.; Merino, J. Llorente; Lou, X.; Mansour, J. D.; Ouyang, Q.; Peng, C.; Ren, H.; Shan, L. Y.; Sun, X.; Xu, D.; Zhu, H.; Zhuang, X.] Chinese Acad Sci, Inst High Energy Phys, Beijing, Peoples R China.
[Gao, J.; Geng, C.; Guo, Y.; Han, L.; Hu, Q.; Jiang, Y.; Li, B.; Li, C.; Liu, J. B.; Liu, M.; Liu, Y. L.; Liu, Y.; Peng, H.; Song, H. Y.; Wang, W.; Zhang, G.; Zhang, R.; Zhao, Z.; Zhu, Y.] Univ Sci & Technol China, Dept Modern Phys, Hefei, Anhui, Peoples R China.
[Chen, S.; Li, L.; Wang, C.; Zhang, H.] Nanjing Univ, Dept Phys, Nanjing, Jiangsu, Peoples R China.
[Du, Y.; Feng, C.; Ma, L. L.; Ma, Y.; Wang, C.; Zhang, X.; Zhao, Y.; Zhu, C. G.] Shandong Univ, Sch Phys, Jinan, Shandong, Peoples R China.
[Bret, M. Cano; Guo, J.; Hu, S.; Yang, H.] Shanghai Jiao Tong Univ, Dept Phys & Astron, Shanghai Key Lab Particle Phys & Cosmol, Shanghai, Peoples R China.
[Chen, X.; Zhou, N.] Tsinghua Univ, Dept Phys, Beijing 100084, Peoples R China.
[Boumediene, D.; Busato, E.; Calvet, D.; Calvet, S.; Chomont, A. R.; Donini, J.; Gris, Ph.; Madar, R.; Pallin, D.; Saez, S. M. Romano; Santoni, C.; Simon, D.; Vazeille, F.] Clermont Univ, Phys Corpusculaire Lab, Clermont Ferrand, France.
[Boumediene, D.; Busato, E.; Calvet, D.; Calvet, S.; Chomont, A. R.; Donini, J.; Gris, Ph.; Madar, R.; Pallin, D.; Saez, S. M. Romano; Santoni, C.; Simon, D.; Vazeille, F.] Univ Blaise Pascal, Clermont Ferrand, France.
[Biebel, O.; Boumediene, D.; Busato, E.; Calvet, D.; Calvet, S.; Chomont, A. R.; Donini, J.; Firan, A.; Gris, Ph.; Madar, R.; Pallin, D.; Saez, S. M. Romano; Santoni, C.; Simon, D.; Vazeille, F.] CNRS IN2P3, Clermont Ferrand, France.
[Alkire, S. P.; Angerami, A.; Brooijmans, G.; Carbone, R. M.; Clark, M. R.; Cole, B.; Hughes, E. W.; Iordanidou, K.; Klein, M. H.; Mohapatra, S.; Ochoa, I.; Parsons, J. A.; Petersen, T. C.; Smith, M. N. K.; Smith, R. W.; Thompson, E. N.; Tuts, P. M.; Wang, T.; Zhou, L.] Columbia Univ, Nevis Lab, Irvington, NY USA.
[Alonso, A.; Besjes, G. J.; Biebel, O.; Dam, M.; Galster, G.; Hansen, J. B.; Hansen, J. D.; Hansen, P. H.; Loevschall-Jensen, A. E.; Monk, J.; Mortensen, S. S.; Pedersen, L. E.; Pingel, A.; Wiglesworth, C.; Xella, S.] Univ Copenhagen, Niels Bohr Inst, Copenhagen, Denmark.
[Cairo, V. M.; Callea, G.; Capua, M.; Crosetti, G.; Del Gaudio, M.; La Rotonda, L.; Mastroberardino, A.; Palazzo, S.; Policicchio, A.; Salvatore, D.; Scarfone, V.; Schioppa, M.; Susinno, G.; Tassi, E.] Univ Calabria, Ist Nazl Fis Nucl, Grp Collegato Cosenza, Lab Nazl Frascati, Arcavacata Di Rende, Italy.
[Cairo, V. M.; Callea, G.; Capua, M.; Crosetti, G.; Del Gaudio, M.; La Rotonda, L.; Palazzo, S.; Policicchio, A.; Salvatore, D.; Scarfone, V.; Schioppa, M.; Susinno, G.; Tassi, E.] Univ Calabria, Dipartimento Fis, Arcavacata Di Rende, Italy.
[Adamczyk, L.; Biebel, O.; Bold, T.; Gach, G. P.; Kisielewska, D.; Koperny, S.; Mindur, B.; Przybycien, M.; Zemla, A.] AGH Univ Sci & Technol, Fac Phys & Appl Comp Sci, Krakow, Poland.
[Palka, M.; Richter-Was, E.] Jagiellonian Univ, Marian Smoluchowski Inst Phys, Krakow, Poland.
[Banas, E.; de Renstrom, P. A. Bruckman; Burka, K.; Chwastowski, J. J.; Derendarz, D.; Godlewski, J.; Gornicki, E.; Hajduk, Z.; Kaczmarska, A.; Knapik, J.; Korcyl, K.; Kowalewska, A. B.; Malecki, Pa.; Olszewski, A.; Olszowska, J.; Stanecka, E.; Staszewski, R.; Trzebinski, M.; Trzupek, A.; Wolter, M. W.; Wosiek, B. K.; Wozniak, K. W.; Zabinski, B.] Polish Acad Sci, Inst Nucl Phys, Krakow, Poland.
[Cao, T.; Firan, A.; Gupta, R.; Hetherly, J. W.; Kama, S.; Kehoe, R.; Sekula, S. J.; Stroynowski, R.; Varol, T.; Wang, H.; Ye, J.; Zhao, X.; Zhou, L.] So Methodist Univ, Dept Phys, Dallas, TX 75275 USA.
[Izen, J. M.; Leyton, M.; Meirose, B.; Namasivayam, H.; Reeves, K.] Univ Texas Dallas, Dept Phys, Richardson, TX 75083 USA.
[Asbah, N.; Behr, J. K.; Bertsche, C.; Bessner, M.; Bloch, I.; Britzger, D.; Deterre, C.; Cornell, S. Diez; Dutta, B.; Dynda, M.; Eckardt, C.; Ferrando, J.; Filipuzzi, M.; Flaschel, N.; Bravo, A. Gascon; Gasnikova, K.; Glazov, A.; Gregor, I. M.; Haleem, M.; Hamnett, P. G.; Hiller, K. H.; Howarth, J.; Huang, Y.; Katzy, J.; Keller, J. S.; Kondrashova, N.; Kuhl, T.; Lobodzinska, E. M.; Lohwasser, K.; Madsen, A.; Medinnis, M.; Moenig, K.; Garcia, R. F. Naranjo; Naumann, T.; O'Rourke, A. A.; Peschke, R.; Peters, K.; Pirumov, H.; Poley, A.; Robinson, J. E. M.; Schaefer, R.; Schmitt, S.; South, D.; Stanescu-Bellu, M.; Stanitzki, M. M.; Styles, N. A.; Tackmann, K.; Trofymov, A.; Wang, J.; Zakharchuk, N.] DESY, Hamburg, Germany.
[Asbah, N.; Behr, J. K.; Bertsche, C.; Bessner, M.; Bloch, I.; Britzger, D.; Deterre, C.; Cornell, S. Diez; Dutta, B.; Dynda, M.; Eckardt, C.; Ferrando, J.; Filipuzzi, M.; Flaschel, N.; Bravo, A. Gascon; Gasnikova, K.; Glazov, A.; Gregor, I. M.; Haleem, M.; Hamnett, P. G.; Hiller, K. H.; Howarth, J.; Huang, Y.; Katzy, J.; Keller, J. S.; Kondrashova, N.; Kuhl, T.; Lobodzinska, E. M.; Lohwasser, K.; Madsen, A.; Medinnis, M.; Moenig, K.; Garcia, R. F. Naranjo; Naumann, T.; O'Rourke, A. A.; Peschke, R.; Peters, K.; Pirumov, H.; Poley, A.; Robinson, J. E. M.; Schaefer, R.; Schmitt, S.; South, D.; Stanescu-Bellu, M.; Stanitzki, M. M.; Styles, N. A.; Tackmann, K.; Trofymov, A.; Wang, J.; Zakharchuk, N.] DESY, Zeuthen, Germany.
[Burmeister, I.; Cinca, D.; Dette, K.; Erdmann, J.; Esch, H.; Goessling, C.; Homann, M.; Klingenberg, R.] Tech Univ Dortmund, Lehrstuhl Expt Phys 4, Dortmund, Germany.
[Anger, P.; Duschinger, D.; Friedrich, F.; Grohs, J. P.; Gutschow, C.; Hauswald, L.; Kobel, M.; Mader, W. F.; Novgorodova, O.; Siegert, F.; Socher, F.; Straessner, A.; Vest, A.; Wahrmund, S.] Tech Univ Dresden, Inst Kern & Teilchenphys, Dresden, Germany.
[Arce, A. T. H.; Benjamin, D. P.; Biebel, O.; Bjergaard, D. M.; Bocci, A.; Cerio, B. C.; Goshaw, A. T.; Kajomovitz, E.; Kotwal, A.; Kruse, M. C.; Li, L.; Li, S.; Liu, M.; Oh, S. H.] Duke Univ, Dept Phys, Durham, NC 27706 USA.
[Bristow, T. M.; Clark, P. J.; Dias, F. A.; Edwards, N. C.; Gao, Y.; Walls, F. M. Garay; Glaysher, P. C. F.; Harrington, R. D.; Leonidopoulos, C.; Martin, V. J.; Mijovic, L.; Mills, C.; Pino, S. A. Olivares; Washbrook, A.; Wynne, B. M.] Univ Edinburgh, SUPA Sch Phys & Astron, Edinburgh, Midlothian, Scotland.
[Antonelli, M.; Beretta, M.; Bilokon, H.; Chiarella, V.; Curatolo, M.; Esposito, B.; Gatti, C.; Laurelli, P.; Maccarrone, G.; Mancini, G.; Sansoni, A.; Testa, M.; Vilucchi, E.] Ist Nazl Fis Nucl, Lab Nazl Frascati, Frascati, Italy.
[Arnold, H.; Betancourt, C.; Boehler, M.; Bruneliere, R.; Buehrer, F.; Burgard, C. D.; Buescher, D.; Cardillo, F.; Coniavitis, E.; Consorti, V.; Dang, N. P.; Dao, V.; Di Simone, A.; Firan, A.; Glatzer, J.; Gonella, G.; Herten, G.; Hirose, M.; Jakobs, K.; Javurek, T.; Jenni, P.; Kiss, F.; Koeneke, K.; Kopp, A. K.; Kuehn, S.; Landgraf, U.; Luedtke, C.; Nagel, M.; Pagacova, M.; Parzefall, U.; Ronzani, M.; Rosbach, K.; Ruehr, F.; Rurikova, Z.; Samme, D.; Schillo, C.; Schnoor, U.; Schumacher, M.; Sommer, P.; Sundermann, J. E.; Ta, D.; Temming, K. K.; Tornambe, P.; Tsiskaridze, V.; Weiser, C.; Werner, M.; Zhang, L.; Zimmermann, S.] Albert Ludwigs Univ, Fak Math & Phys, Freiburg, Germany.
[Ancu, L. S.; De Mendizabal, J. Bilbao; Calace, N.; Chatterjee, A.; Clark, A.; Coccaro, A.; Delitzsch, C. M.; della Volpe, D.; Ferrere, D.; Golling, T.; Gonzalez-Sevilla, S.; Gramling, J.; Guescini, F.; Iacobucci, G.; Katre, A.; Khoo, T. J.; Lanfermann, M. C.; Lionti, A. E.; March, L.; Mermod, P.; Nackenhorst, O.; Paolozzi, L.; Ristic, B.; Schramm, S.; Sfyrla, A.; Wu, X.] Univ Geneva, Sect Phys, Geneva, Switzerland.
[Barberis, D.; Biebel, O.; Darbo, G.; Favareto, A.; Parodi, A. Ferretto; Gagliardi, G.; Gaudiello, A.; Gemme, C.; Guido, E.; Miglioranzi, S.; Morettini, P.; Osculati, B.; Parodi, F.; Passaggio, S.; Rossi, L. P.; Sannino, M.; Schiavi, C.] Univ Genoa, Ist Nazl Fis Nucl, Sez Genova, Genoa, Italy.
[Barberis, D.; Favareto, A.; Parodi, A. Ferretto; Gagliardi, G.; Gaudiello, A.; Guido, E.; Miglioranzi, S.; Osculati, B.; Parodi, F.; Sannino, M.; Schiavi, C.] Univ Genoa, Dipartimento Fis, Genoa, Italy.
[Tskhadadze, E. G.] Iv Javakhishvili Tbilisi State Univ, E Andronikashvili Inst Phys, Tbilisi, Rep of Georgia.
[Djobava, T.; Durglishvili, A.; Khubua, J.; Mosidze, M.] Tbilisi State Univ, Inst High Energy Phys, Tbilisi, Rep of Georgia.
[Dueren, M.; Heinz, C.; Kreutzfeldt, K.; Kroeninger, K.; Stenzel, H.] Justus Liebig Univ Giessen, Phys Inst 2, Giessen, Germany.
[Alshehri, A. A.; Bates, R. L.; Blue, A.; Boutle, S. K.; Madden, W. D. Breaden; Britton, D.; Buckley, A. G.; Bussey, R.; Buttar, C. M.; Buzatu, A.; Crawley, S. J.; D'Auria, S.; Doyle, A. T.; Gul, U.; Knue, A.; Mullen, R.; O'Shea, V.; Owen, M.; Pollard, C. S.; Qin, G.; Quilty, D.; Ravenscroft, T.; Robson, A.; Denis, R. D. St.; Stewart, G. A.; Thompson, A. S.] Univ Glasgow, SUPA Sch Phys & Astron, Glasgow, Lanark, Scotland.
[Agricola, J.; Bindi, M.; Bisanz, T.; Blumenschein, U.; Brandt, G.; De Maria, A.; Drechsler, E.; Graber, L.; Grosse-Knetter, J.; Janus, M.; Kareem, M. J.; Kawamura, G.; Lai, S.; Lemmer, B.; Magradze, E.; Mantoani, M.; Mchedlidze, G.; Llacer, M. Moreno; Musheghyan, H.; Quadt, A.; Rieger, J.; Rosien, N. -A.; Rzehorz, G. F.; Shabalina, E.; Stoke, P.; Veatch, J.; Weingarten, J.; Zinonos, Z.] Georg August Univ, Phys Inst 2, Gottingen, Germany.
[Albrand, S.; Berlendis, S.; Bethani, A.; Camincher, C.; Collot, J.; Crepe-Renaudin, S.; Delsart, P. A.; Gabaldon, C.; Genest, M. H.; Gradin, P. O. J.; Hostachy, J-Y.; Ledroit-Guillon, F.; Lleres, A.; Lucotte, A.; Malek, F.; Petit, E.; Stark, J.; Trocme, B.; Wu, M.] Univ Grenoble Alpes, Lab Phys Subatom & Cosmol, CNRS IN2P3, Grenoble, France.
[Chan, S. K.; Clark, B. L.; Franklin, M.; Giromini, P.; Huth, J.; Ippolito, V.; Lazovich, T.; Mateos, D. Lopez; Morii, M.; Rogan, C. S.; Skottowe, H. P.; Sun, S.; Tolley, E.; Tong, B.; Tuna, A. N.; Yen, A. L.; Zambito, S.] Harvard Univ, Lab Particle Phys & Cosmol, Cambridge, MA 02138 USA.
[Andrei, V.; Antel, C.; Baas, A. E.; Brandt, O.; Djuvsland, J. I.; Dunford, M.; Geisler, M. P.; Hanke, R.; Jongmanns, J.; Kluge, E. -E.; Lang, V. S.; Meier, K.; Zu Theenhausen, H. Meyer; Villar, D. I. Narrias; Sahinsoy, M.; Scharf, V.; Schultz-Coulon, H. -C.; Stamen, R.; Starovoitov, P.; Suchek, S.; Wessels, M.] Heidelberg Univ, Kirchhoff Inst Phys, Heidelberg, Germany.
[Anders, C. F.; de Lima, D. E. Ferreira; Kolb, M.; Lisovyi, M.; Schaetzel, S.; Schoening, A.; Sosa, D.] Heidelberg Univ, Inst Phys, Heidelberg, Germany.
[Anders, C. F.; de Lima, D. E. Ferreira; Kolb, M.; Lisovyi, M.; Schaetzel, S.; Schoening, A.; Sosa, D.] Heidelberg Univ, ZITI Inst Tech Informat, Mannheim, Germany.
[Nagasaka, Y.] Hiroshima Inst Technol, Fac Appl Informat Sci, Hiroshima, Japan.
[Bortolotto, V.; Chan, Y. L.; Castillo, L. R. Flores; Lu, H.; Salvucci, A.; Tsui, K. M.] Chinese Univ Hong Kong, Dept Phys, Shatin, Hong Kong, Peoples R China.
[Bortolotto, V.; Orlando, N.; Tu, Y.] Univ Hong Kong, Dept Phys, Hong Kong, Hong Kong, Peoples R China.
[Bortolotto, V.; Prokofiev, K.] Hong Kong Univ Sci & Technol, Dept Phys, Clear Water Bay, Kowloon, Hong Kong, Peoples R China.
[Choi, K.; Dattagupta, A.; Evans, H.; Gagnon, P.; Kopeliansky, R.; Lammers, S.; Martinez, N. Lorenzo; Luehring, F.; Ogren, H.; Penwell, J.; Weinert, B.; Zieminska, D.] Indiana Univ, Dept Phys, Bloomington, IN 47405 USA.
[Guenther, J.; Iwanski, W.; Jansky, R.; Kneringer, E.; Lukas, W.; Milic, A.] Leopold Franzens Univ, Inst Astro & Teilchenphys, Innsbruck, Austria.
[Abdallah, J.; Argyropoulos, S.; Benitez, J.; Zaidan, R.] Univ Iowa, Iowa City, IA USA.
[Chen, C.; Cochran, J.; De Lorenzi, F.; Jiang, H.; Krumnack, N.; Pluth, D.; Prell, S.; Werner, M. D.; Yu, J.] Iowa State Univ, Dept Phys & Astron, Ames, IA USA.
[Ahmadov, F.; Biebel, O.; Chelkov, G. A.; Cheplakov, A.; Dedovich, D. V.; Gongadze, A.; Khramov, E.; Ladygin, E.; Plotnikova, E.; Sapronov, A.; Soloshenko, A.; Zhemchugov, A.] JINR Dubna, Joint Inst Nucl Res, Dubna, Russia.
[Amako, K.; Aoki, M.; Arai, Y.; Hanagaki, K.; Honda, T.; Ikegami, Y.; Ikeno, M.; Iwasaki, H.; Kanzaki, J.; Kondo, T.; Kono, T.; Makida, Y.; Mallik, U.; Nagai, R.; Nagano, K.; Nakamura, K.; Nozaki, M.; Odaka, S.; Okuyama, T.; Sasaki, O.; Suzuki, S.; Takubo, Y.; Tanaka, S.; Terada, S.; Tokushuku, K.; Tsuno, S.; Unno, Y.; Yamamoto, A.; Yasu, Y.] KEK, High Energy Accelerator Res Org, Tsukuba, Ibaraki, Japan.
[Biebel, O.; Chen, Y.; Hasegawa, M.; Kido, S.; Kurashige, H.; Maeda, J.; Ochi, A.; Shimizu, S.; Tanioka, R.; Yamazaki, Y.; Yuan, L.] Kobe Univ, Grad Sch Sci, Kobe, Hyogo, Japan.
[Kunigo, T.; Monden, R.; Sumida, T.; Tashiro, T.] Kyoto Univ, Fac Sci, Kyoto, Japan.
[Takashima, R.] Kyoto Univ, Kyoto, Japan.
[Biebel, O.; Kawagoe, K.; Oda, S.; Otono, H.; Shirabe, S.; Tojo, J.] Kyushu Univ, Dept Phys, Fukuoka, Japan.
[Verzini, M. J. Alconada; Alonso, F.; Arduh, F. A.; Dova, M. T.; Hoya, J.; Monticelli, F.; Wahlberg, H.] Univ Nacl La Plata, Inst Fis La Plata, La Plata, Buenos Aires, Argentina.
[Verzini, M. J. Alconada; Alonso, F.; Arduh, F. A.; Dova, M. T.; Hoya, J.; Monticelli, F.; Wahlberg, H.] Consejo Nacl Invest Cient & Tecn, La Plata, Buenos Aires, Argentina.
[Barton, A. E.; Beattie, M. D.; Bertram, I. A.; Borissov, G.; Bouhova-Thacker, E. V.; Dearnaley, W. J.; Fox, H.; Grimm, K.; Henderson, R. C. W.; Hughes, G.; Jones, R. W. L.; Kartvelishvili, V.; Long, R. E.; Love, P. A.; Muenstermann, D.; Parker, A. J.; Skinner, M. B.; Smizanska, M.; Walder, J.; Wharton, A. M.] Univ Lancaster, Dept Phys, Lancaster, England.
[Aliev, M.; Bachas, K.; Chiodini, G.; Gorini, E.; Longo, L.; Primavera, M.; Reale, M.; Spagnolo, S.; Ventura, A.] Univ Salento, Ist Nazl Fis Nucl, Sez Lecce, Lecce, Italy.
[Aliev, M.; Bachas, K.; Gorini, E.; Longo, L.; Reale, M.; Spagnolo, S.; Ventura, A.] Univ Salento, Dipartimento Matemat & Fis, Lecce, Italy.
[Affolder, A. A.; Anders, J. K.; Burdin, S.; D'Onofrio, M.; Dervan, P.; Gwilliam, C. B.; Hayward, H. S.; Jones, T. J.; King, B. T.; Klein, M.; Klein, U.; Kretzschmar, J.; Laycock, P.; Lehan, A.; Maxfield, S. J.; Mehta, A.; Readioff, N. P.; Vossebeld, J. H.] Univ Liverpool, Oliver Lodge Lab, Liverpool, Merseyside, England.
[Cindro, V.; Filipcic, A.; Gorisek, A.; Kanjir, L.; Kersevan, B. P.; Kramberger, G.; Macek, B.; Mandic, I.; Mikuz, M.; Muskinja, M.; Sfiligoj, T.; Sokhrannyi, G.] Jozef Stefan Inst, Dept Phys, Ljubljana, Slovenia.
[Cindro, V.; Filipcic, A.; Gorisek, A.; Kanjir, L.; Kersevan, B. P.; Kramberger, G.; Macek, B.; Mandic, I.; Mikuz, M.; Muskinja, M.; Sfiligoj, T.; Sokhrannyi, G.] Univ Ljubljana, Ljubljana, Slovenia.
[Armitage, L. J.; Bevan, A. J.; Biebel, O.; Bona, M.; Hays, J. M.; Hickling, R.; Landon, M. P. J.; Lewis, D.; Lloyd, S. L.; Morris, J. D.; Nooney, T.; Piccaro, E.; Rizvi, E.; Sandbach, R. L.] Queen Mary Univ London, Sch Phys & Astron, London, England.
[Berry, T.; Boisvert, V.; Brooks, T.; Connelly, I. A.; Cowan, G.; Giannelli, M. Faucci; Gadomski, S.; George, S.; Gibson, S. M.; Kempster, J. J.; Kilby, C. R.; Vazquez, J. G. Panduro; Pastore, Fr.; Savage, G.; Sowden, B. C.; Spano, F.; Teixeira-Dias, R.; Thomas-Wilsker, J.] Royal Holloway Univ London, Dept Phys, Surrey, England.
[Bell, A. S.; Butterworth, J. M.; Campanelli, M.; Christodoulou, V.; Cooper, B. D.; Davison, P.; Falla, R. J.; Freeborn, D.; Gregersen, K.; Grout, Z. J.; Ortiz, N. G. Gutierrez; Hesketh, G. G.; Jiggins, S.; Konstantinidis, N.; Korn, A.; Kucuk, H.; Leney, K. J. C.; Martyniuk, A. C.; McClymont, L. I.; Mcfayden, J. A.; Nurse, E.; Richter, S.; Scanlon, T.; Sherwood, P.; Simmons, B.; Wardrope, D. R.; Waugh, B. M.] UCL, Dept Phys & Astron, London, England.
[Greenwood, Z. D.; Grossi, G. C.; Jana, D. K.; Sawyer, L.] Louisiana Tech Univ, Ruston, LA 71270 USA.
[Beau, T.; Bomben, M.; Calderini, G.; Crescioli, F.; De Cecco, S.; Demilly, A.; Derue, F.; Francavilla, P.; Krasny, M. W.; Lacour, D.; Laforge, B.; Laplace, S.; Le Dortz, O.; Lefebvre, G.; Solis, A. Lopez; Luzi, P. M.; Malaescu, B.; Marchiori, G.; Nikolic-Audit, I.; Ocariz, J.; Pandini, C. E.; Pires, S.; Ridel, M.; Roos, L.; Trincaz-Duvoid, S.; Varouchas, D.; Yap, Y. C.] UPMC, Lab Phys Nucl & Hautes Energies, Paris, France.
[Beau, T.; Bomben, M.; Calderini, G.; Crescioli, F.; De Cecco, S.; Demilly, A.; Derue, F.; Francavilla, P.; Krasny, M. W.; Lacour, D.; Laforge, B.; Laplace, S.; Le Dortz, O.; Lefebvre, G.; Solis, A. Lopez; Luzi, P. M.; Malaescu, B.; Marchiori, G.; Nikolic-Audit, I.; Ocariz, J.; Pandini, C. E.; Pires, S.; Ridel, M.; Roos, L.; Trincaz-Duvoid, S.; Varouchas, D.; Yap, Y. C.] Univ Paris Diderot, Paris, France.
[Beau, T.; Bomben, M.; Calderini, G.; Crescioli, F.; De Cecco, S.; Demilly, A.; Derue, F.; Francavilla, P.; Krasny, M. W.; Lacour, D.; Laforge, B.; Laplace, S.; Le Dortz, O.; Lefebvre, G.; Solis, A. Lopez; Luzi, P. M.; Malaescu, B.; Marchiori, G.; Nikolic-Audit, I.; Ocariz, J.; Pandini, C. E.; Pires, S.; Ridel, M.; Roos, L.; Trincaz-Duvoid, S.; Varouchas, D.; Yap, Y. C.] CNRS IN2P3, Paris, France.
[Akesson, T. P. A.; Bocchetta, S. S.; Bryngemark, L.; Doglioni, C.; Hedberg, V.; Jarlskog, G.; Lytken, E.; Mjornmark, J. U.; Smirnova, O.; Viazlo, O.] Lund Univ, Fys Inst, Lund, Sweden.
[Barreiro, F.; Calvente Lopez, S.; Cueto, A.; Del Peso, J.; Glasman, C.; Terron, J.] Univ Autonoma Madrid, Dept Fis Teor C 15, Madrid, Spain.
[Artz, S.; Becker, M.; Bertella, C.; Blum, W.; Buescher, V.; Cuth, J.; Dudder, A. Chr.; Endner, O. C.; Ertel, E.; Fiedler, F.; Torregrosa, E. Fullana; Geisen, M.; Groh, S.; Heck, T.; Jakobi, K. B.; Kaluza, A.; Karnevskiy, M.; Kleinknecht, K.; Koepke, L.; Lin, T. H.; Masetti, L.; Mattmann, J.; Meyer, C.; Moritz, S.; Pleskot, V.; Rave, S.; Reiss, A.; Sander, H. G.; Schaeffer, J.; Schaefer, U.; Schmitt, C.; Schmitz, S.; Schott, M.; Schuh, N.; Schulte, A.; Simioni, E.; Simon, M.; Tapprogge, S.; Urrejola, P.; Webb, S.; Yildirim, E.; Zimmermann, C.; Zinser, M.] Johannes Gutenberg Univ Mainz, Inst Phys, Mainz, Germany.
[Barnes, S. L.; Bielski, R.; Cox, B. E.; Da Via, C.; Dann, N. S.; Forcolin, G. T.; Forti, A.; Ponce, J. M. Iturbe; Li, X.; Loebinger, F. K.; Marsden, S. P.; Masik, J.; Sanchez, F. J. Munoz; Neep, T. J.; Oh, A.; Ospanov, R.; Pater, J. R.; Peters, R. F. Y.; Pilkington, A. D.; Pin, A. W. J.; Price, D.; Qin, Y.; Queitsch-Maitland, M.; Raine, J. A.; Schweiger, H.; Shaw, S. M.; Tomlinson, L.; Watts, S.; Wilk, F.; Woudstra, M. J.; Wyatt, T. R.] Univ Manchester, Sch Phys & Astron, Manchester, Lancs, England.
[Aad, G.; Alstaty, M.; Barbero, M.; Brennan, A. J.; Calandri, A.; Calvet, T. P.; Coadou, Y.; Diaconu, C.; Djama, F.; Ellajosyula, V.; Feligioni, L.; Hadef, A.; Hallewel, G. D.; Hubaut, F.; Kahn, S. J.; Knoops, E. B. F. G.; Le Guirriec, E.; Liu, J.; Liu, K.; Monnier, E.; Muanza, S.; Nagy, E.; Pralavorio, P.; Rodina, Y.; Rozanov, A.; Talby, M.; Taylor, G. N.; Taylor, P. T. E.; Theveneaux-Pelzer, T.; Torres, R. E. Ticse; Tisserant, S.; Toth, J.; Touchard, F.; Vacavant, L.; Wang, C.] Aix Marseille Univ, CPPM, Marseille, France.
[Aad, G.; Alstaty, M.; Barbero, M.; Brennan, A. J.; Calandri, A.; Calvet, T. P.; Coadou, Y.; Diaconu, C.; Djama, F.; Ellajosyula, V.; Feligioni, L.; Firan, A.; Hadef, A.; Hallewel, G. D.; Hubaut, F.; Kahn, S. J.; Knoops, E. B. F. G.; Le Guirriec, E.; Liu, J.; Liu, K.; Monnier, E.; Muanza, S.; Nagy, E.; Pralavorio, P.; Rodina, Y.; Rozanov, A.; Talby, M.; Taylor, G. N.; Taylor, P. T. E.; Theveneaux-Pelzer, T.; Torres, R. E. Ticse; Tisserant, S.; Toth, J.; Touchard, F.; Vacavant, L.; Wang, C.] CNRS IN2P3, Marseille, France.
[Bellomo, M.; Bernard, N. R.; Brau, B.; Dallapiccola, C.; Moyse, E. J. W.; Pais, R.; Pettersson, N. E.; Picazio, A.; Willocq, S.] Univ Massachusetts, Dept Phys, Amherst, MA 01003 USA.
[Belanger-Champagne, C.; Chuinard, A. J.; Corriveau, F.; Keyes, R. A.; Lefebvre, B.; Mantifel, R.; Prince, S.; Robertson, S. H.; Robichaud-Veronneau, A.; Stockton, M. C.; Stoebe, M.; Vachon, B.; Schroeder, T. Vazquez; Wang, K.] McGill Univ, Dept Phys, Montreal, PQ, Canada.
[Barberio, E. L.; Dawe, E.; Goldfarb, S.; Jennens, D.; Kubota, T.; Le, B.; McDonald, E. F.; Milesi, M.; Nuti, F.; Rados, P.; Scutti, F.; Spiller, L. A.; Tan, K. G.; Ungaro, F. C.; Urquijo, P.; Volpi, M.; Zanzi, D.] Univ Melbourne, Sch Phys, Melbourne, Vic, Australia.
[Amidei, D.; Chelstowska, M. A.; Cheng, H. C.; Dai, T.; Diehl, E. B.; Edgar, R. C.; Feng, H.; Ferretti, C.; Fleischmann, R.; Guan, L.; Levin, D.; Liu, H.; Lu, N.; Marley, D. E.; Mc Kee, S. P.; McCarnn, A.; Neal, H. A.; Qian, J.; Schwarz, T. A.; Searcy, J.; Sekhon, K.; Wu, Y.; Yu, J. M.; Zhang, D.; Zhou, B.; Zhu, J.] Univ Michigan, Dept Phys, Ann Arbor, MI 48109 USA.
[Arabidze, G.; Brock, R.; Chegwidden, A.; De la Torre, H.; Fisher, W. C.; Halladjian, G.; Hauser, R.; Hayden, D.; Huston, J.; Martin, B.; Mondragon, M. C.; Plucinski, P.; Pope, B. G.; Schoenrock, B. D.; Schwienhorst, R.; Willis, C.] Michigan State Univ, Dept Phys & Astron, E Lansing, MI 48824 USA.
[Alimonti, G.; Andreazza, A.; Camplani, A.; Carminati, L.; Cavalli, D.; Citterio, M.; Costa, G.; Fanti, M.; Giugni, D.; Lari, T.; Lazzaroni, M.; Mandelli, L.; Manzoni, S.; Mazza, S. M.; Meroni, C.; Monzani, S.; Perini, L.; Ragusa, F.; Ratti, M. G.; Resconi, S.; Shojaii, S.; Stabile, A.; Tartarelli, G. F.; Troncon, C.; Turra, R.; Perez, M. Villaplana] Univ Milan, Ist Nazl Fis Nucl, Sez Milano, Milan, Italy.
[Andreazza, A.; Camplani, A.; Carminati, L.; Fanti, M.; Lazzaroni, M.; Manzoni, S.; Mazza, S. M.; Monzani, S.; Perini, L.; Ragusa, F.; Ratti, M. G.; Shojaii, S.; Turra, R.; Perez, M. Villaplana] Univ Milan, Dipartimento Fis, Milan, Italy.
[Harkusha, S.; Kulchitsky, Y.; Kurochkin, Y. A.; Tsiareshka, P. V.] Natl Acad Sci Belarus, BI Stepanov Inst Phys, Minsk, Byelarus.
[Hrynevich, A.] Natl Sci & Educ Ctr Particle & High Energy Phys, Minsk, Byelarus.
[Arguin, J-F.; Azuelos, G.; Biebel, O.; Billoud, T. R. V.; Dallaire, F.; Ducu, O. A.; Gagnon, L. G.; Gauthier, L.; Leroy, C.; Mochizuki, K.; Manh, T. Nguyen; Rezvani, R.; Saadi, D. Shoaleh] Univ Montreal, Grp Particle Phys, Montreal, PQ, Canada.
[Akimov, A. V.; Gavrilenko, I. L.; Komar, A. A.; Madaffari, D.; Mashinistov, R.; Nechaeva, P. Yu.; Shmeleva, A.; Snesarev, A. A.; Sulin, V. V.; Tikhomirov, V. O.; Zhukov, K.] Russian Acad Sci, PN Lebedev Phys Inst, Moscow, Russia.
[Artamonov, A.; Gorbounov, P. A.; Khovanskiy, V.; Shatalov, P. B.; Tsukerman, I. I.] Inst Theoret & Expt Phys ITEP, Moscow, Russia.
[Antonov, A.; Belotskiy, K.; Belyaev, N. L.; Bulekov, O.; Kantserov, V. A.; Krasnopevtsev, D.; Romaniouk, A.; Shulga, E.; Smirnov, S. Yu.; Smirnov, Y.; Soldatov, E. Yu.; Timoshenko, S.; Vorobev, K.] Natl Res Nucl Univ MEPhI, Moscow, Russia.
[Gladilin, L. K.; Kramarenko, V. A.; Maevskiy, A.; Sivoklokov, S. Yu.; Smirnova, L. N.] Moscow MV Lomonosov State Univ, DV Skobeltsyn Inst Nucl Phys, Moscow, Russia.
[Adomeit, S.; Bender, M.; Biebel, O.; Bock, C.; Calfayan, P.; Chow, B. K. B.; Duckeck, G.; Hartmann, N. M.; Heinrich, J. J.; Hertenberger, R.; Hoenig, F.; Legger, F.; Lorenz, J.; Loesel, P. J.; Maier, T.; Mann, A.; Mehlhase, S.; Meineck, C.; Mitrevski, J.; Mueller, R. S. P.; Rauscher, F.; Ruschke, A.; Schachtner, B. M.; Schaile, D.; Unverdorben, C.; Valderanis, C.; Walker, R.; Wittkowski, J.] Ludwig Maximilians Univ Munchen, Fak Phys, Munich, Germany.
[Barillari, T.; Bethke, S.; Biebel, O.; Compostella, G.; Cortiana, G.; Ecker, K. M.; Flowerdew, M. J.; Giuliani, C.; Ince, T.; Kiryunin, A. E.; Kluth, S.; Koehler, N. M.; Kortner, O.; Kortner, S.; Kroha, H.; La Rosa, A.; Macchiolo, A.; Maier, A. A.; McCarthy, T. G.; Menke, S.; Mueller, F.; Nisius, R.; Nowak, S.; Oberlack, H.; Richter, R.; Salihagic, D.; Savic, N.; Schacht, P.; Schmidt-Sommerfeld, K. R.; Spettel, F.; Stonjek, S.; von der Schmitt, H.; Wildauer, A.] Werner Heisenberg Inst, Max Planck Inst Phys, Munich, Germany.
[Fusayasu, T.; Shimojima, M.] Nagasaki Inst Appl Sci, Nagasaki, Japan.
[Horii, Y.; Kentaro, K.; Nakahama, Y.; Onogi, K.; Tomoto, M.; Wakabayashi, J.; Yamauchi, K.] Nagoya Univ, Grad Sch Sci, Nagoya, Aichi, Japan.
[Horii, Y.; Kentaro, K.; Nakahama, Y.; Onogi, K.; Tomoto, M.; Wakabayashi, J.; Yamauchi, K.] Nagoya Univ, Kobayashi Maskawa Inst, Nagoya, Aichi, Japan.
[Aloisio, A.; Alviggi, M. G.; Canale, V.; Carlino, G.; Cirotto, F.; Conventi, F.; de Asmundis, R.; Della Pietra, M.; Doria, A.; Izzo, V.; Merola, L.; Perrella, S.; Rossi, E.; Sanchez, A.; Sekhniaidze, G.] Univ Napoli, Sez Napoli, Ist Nazl Fis Nucl, Naples, Italy.
[Aloisio, A.; Alviggi, M. G.; Canale, V.; Cirotto, F.; Merola, L.; Perrella, S.; Rossi, E.; Sanchez, A.] Univ Napoli, Dipartimento Fis, Naples, Italy.
[Gorelov, I.; Hoeferkamp, M. R.; Mc Fadden, N. C.; Seidel, S. C.; Taylor, A. C.; Toms, K.] Univ New Mexico, Dept Phys & Astron, Albuquerque, NM 87131 USA.
[Biebel, O.; Caron, S.; Colasurdo, L.; Croft, V.; De Groot, N.; Filthaut, F.; Galea, C.; Koenig, A. C.; Nektarijevic, S.; Strubig, A.] Radboud Univ Nijmegen Nikhef, Inst Math Astrophys & Particle Phys, Nijmegen, Netherlands.
[Aben, R.; Angelozzi, I.; Bedognetti, M.; Beemster, L. J.; Bentvelsen, S.; Berge, D.; Biebel, O.; Bobbink, G. J.; Bos, K.; Brenner, L.; Bruni, L. S.; Butti, P.; Castelijn, R.; Castelli, A.; Colijn, A. P.; de Jong, P.; Deigaard, I.; Duda, D.; Ferrari, P.; Firan, A.; Hartjes, F.; Hessey, N. P.; Igonkina, O.; Kluit, R.; Koffeman, E.; Mahlstedt, J.; Maio, A.; Meyer, J.; Oussoren, K. P.; Sabato, G.; Salek, D.; Slawinska, M.; Valencic, N.; Van Den Wollenberg, W.; Van Der Deijl, P. C.; van der Graaf, H.; van Vulpen, I.; Vankov, P.; Verkerke, W.; Vermeulen, J. C.; Vreeswijk, M.; Weits, H.; Williams, S.; Wolf, T. M. H.] Nikhef Natl Inst Subatom Phys, Amsterdam, Netherlands.
[Aben, R.; Angelozzi, I.; Bedognetti, M.; Beemster, L. J.; Bentvelsen, S.; Berge, D.; Biebel, O.; Bobbink, G. J.; Bos, K.; Brenner, L.; Bruni, L. S.; Butti, P.; Castelijn, R.; Castelli, A.; Colijn, A. P.; de Jong, P.; Deigaard, I.; Duda, D.; Ferrari, P.; Firan, A.; Hartjes, F.; Hessey, N. P.; Igonkina, O.; Kluit, R.; Koffeman, E.; Mahlstedt, J.; Meyer, J.; Oussoren, K. P.; Sabato, G.; Salek, D.; Slawinska, M.; Valencic, N.; Van Den Wollenberg, W.; Van Der Deijl, P. C.; van der Graaf, H.; van Vulpen, I.; Vankov, P.; Verkerke, W.; Vermeulen, J. C.; Vreeswijk, M.; Weits, H.; Williams, S.; Wolf, T. M. H.] Univ Amsterdam, Amsterdam, Netherlands.
[Adelman, J.; Brost, E.; Burghgrave, B.; Chakraborty, D.; Klimek, R.; Saha, P.] No Illinois Univ, Dept Phys, De Kalb, IL 60115 USA.
[Anisenkov, A. V.; Baldin, E. M.; Bobrovnikov, V. S.; Bogdanchikov, A. G.; Buzykaev, A. R.; Kazanin, V. F.; Kharlamov, A. G.; Kharlamova, T.; Korol, A. A.; Maslennikov, A. L.; Maximov, D. A.; Peleganchuk, S. V.; Rezanova, O. L.; Soukharev, A. M.; Talyshev, A. A.; Tikhonov, Yu. A.] SB RAS, Budker Inst Nucl Phys, Novosibirsk, Russia.
[Becot, C.; Bernius, C.; Biebel, O.; Cranmer, K.; Haas, A.; Heinrich, L.; Kaplan, B.; Karthik, K.; Konoplich, R.; Mincer, A. I.; Nemethy, R.; Neves, R. M.] NYU, Dept Phys, 4 Washington Pl, New York, NY 10003 USA.
[Beacham, J. B.; Che, S.; Gan, K. K.; Ishmukhametov, R.; Kagan, H.; Kass, R. D.; Looper, K. A.; Shrestha, S.; Tannenwald, B. B.] Ohio State Univ, Columbus, OH 43210 USA.
[Nakano, I.] Okayama Univ, Fac Sci, Okayama, Japan.
[Abbott, B.; Alhroob, M.; Bertsche, D.; De Benedetti, A.; Gutierrez, P.; Hasib, A.; Norberg, S.; Pearson, B.; Rifki, O.; Severini, H.; Shope, D. R.; Skubic, P.; Strauss, M.] Univ Oklahoma, Homer L Dodge Dept Phys & Astron, Norman, OK 73019 USA.
[Cantero, J.; Haley, J.; Jamin, D. O.; Khanov, A.; Rizatdinova, F.; Sidorov, D.] Oklahoma State Univ, Dept Phys, Stillwater, OK 74078 USA.
[Chytka, L.; Hamal, R.; Hrabovsky, M.; Kvita, J.; Nozka, L.] Palacky Univ, RCPTM, Olomouc, Czech Republic.
[Abreu, R.; Allen, B. W.; Biebel, O.; Brau, J. E.; Firan, A.; Hopkins, W. H.; Majewski, S.; Potter, C. T.; Radloff, P.; Sinev, N. B.; Snyder, I. M.; Strom, D. M.; Torrence, E.; Wanotayaroj, C.; Whalen, K.; Winklmeier, F.] Univ Oregon, Ctr High Energy Phys, Eugene, OR 97403 USA.
[Abeloos, B.; Ayoub, M. K.; Bassalat, A.; Binet, S.; Bourdarios, C.; De Regie, J. B. De Vivie; Delgove, D.; Duflot, L.; Escalier, M.; Fayard, L.; Fournier, D.; Gkougkousis, E. L.; Goudet, C. R.; Grivaz, J. -F.; Hariri, F.; Henrot-Versille, S.; Hrivnac, J.; Iconomidou-Fayard, L.; Kado, M.; Lounis, A.; Maiani, C.; Makovec, N.; Morange, N.; Nellist, C.; Petroff, P.; Poggioli, L.; Puzo, P.; Rousseau, D.; Rybkin, G.; Schaffer, A. C.; Serin, L.; Simion, S.; Tanaka, R.; Zerwas, D.; Zhang, Z.] Univ Paris Saclay, Univ Paris Sud, LAL, CNRS IN2P3, Orsay, France.
[Ishijima, N.; Nomachi, M.; Sugaya, Y.; Teoh, J. J.; Yamaguchi, Y.] Osaka Univ, Grad Sch Sci, Osaka, Japan.
[Bugge, M. K.; Cameron, D.; Catmore, J. R.; Feigl, S.; Franconi, L.; Garonne, V.; Gjelsten, B. K.; Gramstad, E.; Morisbak, V.; Nilsen, J. K.; Ould-Saada, F.; Pajchel, K.; Pedersen, M.; Raddum, S.; Read, A. L.; Rohne, O.; Sandaker, H.; Serfon, C.; Stapnes, S.; Strandlie, A.] Univ Oslo, Dept Phys, Oslo, Norway.
[Artoni, G.; Backes, M.; Barr, A. J.; Becker, K.; Beresford, L.; Bortoletto, D.; Burr, J. T. P.; Cooper-Sarkar, A. M.; Ortuzar, M. Crispin; Fawcett, W. J.; Frost, J. A.; Gallas, E. J.; Giuli, F.; Gupta, S.; Gwenlan, C.; Hays, C. P.; Henderson, J.; Huffman, T. B.; Issever, C.; Kalderon, C. W.; Nagai, K.; Nickerson, R. B.; Norjoharuddeen, N.; Petrov, M.; Pickering, M. A.; Radescu, V.; Tseng, J. C-L.; Viehhauser, G. H. A.; Vigani, L.; Weidberg, A. R.; Zhong, J.] Univ Oxford, Dept Phys, Oxford, England.
[Farina, E. M.; Ferrari, R.; Fraternali, M.; Gaudio, G.; Introzzi, G.; Kourkoumeli-Charalampidi, A.; Lanza, A.; Livan, M.; Negri, A.; Polesello, G.; Rebuzzi, D. M.; Rimoldi, A.; Vercesi, V.] Univ Pavia, Sez Pavia, Ist Nazl Fis Nucl, Pavia, Italy.
[Dondero, R.; Farina, E. M.; Fraternali, M.; Introzzi, G.; Kourkoumeli-Charalampidi, A.; Livan, M.; Negri, A.; Rebuzzi, D. M.; Rimoldi, A.] Univ Pavia, Dipartimento Fis, Pavia, Italy.
[Balunas, W. K.; Brendlinger, K.; Di Clemente, W. K.; Fletcher, R. R. M.; Haney, B.; Heim, S.; Hines, E.; Jackson, B.; Kroll, J.; Lipeles, E.; Miguens, J. Machado; Meyer, C.; Mistry, K. P.; Reichert, J.; Schaefer, L.; Thomson, E.; Vanguri, R.; Williams, H. H.; Yoshihara, K.] Univ Penn, Dept Phys, Philadelphia, PA 19104 USA.
[Basalaev, A.; Biebel, O.; Ezhilov, A.; Fedin, O. L.; Gratchev, V.; Levchenko, M.; Maleev, V. P.; Naryshkin, I.; Ryabov, Y. F.; Schegelsky, V. A.; Seliverstov, D. M.; Solovyev, V.] BP Konstantinov Petersburg Nucl Phys Inst, Kurchatov Inst, Natl Res Ctr, St Petersburg, Russia.
[Annovi, A.; Bertolucci, E.; Biesuz, N. V.; Cavasinni, V.; Chiarelli, G.; Del Prete, T.; Dell'Orso, M.; Donati, S.; Dondero, R.; Giannetti, P.; Leone, S.; Roda, C.; Scuri, F.; Sotiropoulou, C. L.; Spalla, M.; Volpi, G.] Univ Pisa, Sez Pisa, Ist Nazl Fis Nucl, Pisa, Italy.
[Annovi, A.; Bertolucci, E.; Biesuz, N. V.; Cavasinni, V.; Chiarelli, G.; Del Prete, T.; Dell'Orso, M.; Donati, S.; Giannetti, P.; Leone, S.; Roda, C.; Scuri, F.; Sotiropoulou, C. L.; Spalla, M.; Volpi, G.] Univ Pisa, Dipartimento Fis E Fermi, Pisa, Italy.
[Bianchi, R. M.; Boudreau, J.; Escobar, C.; Farina, C.; Hong, T. M.; Mueller, J.; Sapp, K.; Su, J.] Univ Pittsburgh, Dept Phys & Astron, Pittsburgh, PA 15260 USA.
[Aguilar-Saavedra, J. A.; Amor Dos Santos, S. P.; Amorim, A.; Araque, J. P.; Carvalho, J.; Castro, N. F.; Conde Muinoa, P.; Da Cunha Sargedas De Sousa, M. J.; Fiolhais, M. C. N.; Galhardo, B.; Gomes, A.; Goncalo, R.; Jorge, P. M.; Maio, A.; Maneira, J.; Seabra, L. F. Oleiro; Onofre, A.; Pedro, R.; Santos, H.; Saraiva, J. G.; Silva, J.; Tavares Delgado, A.; Veloso, F.; Wolters, H.] LIP, Lab Instrumentactio & Fis Expt Particulas, Lisbon, Portugal.
[Amorim, A.; Conde Muinoa, P.; Da Cunha Sargedas De Sousa, M. J.; Gomes, A.; Jorge, P. M.; Miguens, J. Machado; Maio, A.; Maneira, J.; Pedro, R.; Tavares Delgado, A.] Univ Lisbon, Fac Ciencias, Lisbon, Portugal.
[Amor Dos Santos, S. P.; Carvalho, J.; Fiolhais, M. C. N.; Galhardo, B.; Veloso, F.; Wolters, H.] Univ Coimbra, Dept Phys, Coimbra, Portugal.
[Gomes, A.; Maio, A.; Saraiva, J. G.; Silva, J.] Univ Lisbon, Ctr Fis Nucl, Lisbon, Portugal.
[Onofre, A.] Univ Minho, Dept Fis, Braga, Portugal.
[Aguilar-Saavedra, J. A.] Univ Granada, Dept Fis Teor & Cosmos, Granada, Spain.
[Aguilar-Saavedra, J. A.] Univ Granada, CAFPE, Granada, Spain.
Univ Nova Lisboa, Fac Ciencias & Tecnol, Dep Fis, Caparica, Portugal.
Univ Nova Lisboa, Fac Ciencias & Tecnol, CEFITEC, Caparica, Portugal.
[Chudoba, J.; Havranek, M.; Hejbal, J.; Jakoubek, T.; Kepka, O.; Kupco, A.; Kus, V.; Lokajicek, M.; Lysak, R.; Marcisovsky, M.; Mikestikova, M.; Nemecek, S.; Penc, O.; Sicho, P.; Staroba, P.; Svatos, M.; Tasevsky, M.; Vrba, V.] Acad Sci Czech Republic, Inst Phys, Prague, Czech Republic.
[Ali, B.; Augsten, K.; Caforio, D.; Gallus, P.; Hubacek, Z.; Myska, M.; Pospisil, S.; Seifert, F.; Simak, V.; Slavicek, T.; Smolek, K.; Solar, M.; Sopczak, A.; Sopko, V.; Suk, M.; Turecek, D.; Vacek, V.; Vlasak, M.; Vokac, P.; Vykydal, Z.; Zeman, M.] Czech Tech Univ, Prague, Czech Republic.
[Berta, R.; Carli, I.; Davidek, T.; Dolejsi, J.; Dolezal, Z.; Kodys, P.; Kosek, T.; Leitner, R.; Mlynarikova, M.; Reznicek, P.; Scheirich, D.; Slovak, R.; Spousta, M.; Sykora, T.; Tas, P.; Todorova-Nova, S.; Valkar, S.; Vorobel, V.] Charles Univ Prague, Fac Math & Phys, Prague, Czech Republic.
[Borisov, A.; Cheremushkina, E.; Denisov, S. P.; Fakhrutdinov, R. M.; Fenyuk, A. B.; Golubkov, D.; Kamenshchikov, A.; Karyukhin, A. N.; Kozhin, A. S.; Minaenko, A. A.; Myagkov, A. G.; Nikolaenko, V.; Ryzhov, A.; Solodkov, A. A.; Solovyanov, O. V.; Starchenko, E. A.; Vaniachine, A.; Zaitsev, A. M.; Zenin, O.] NRC KI, State Res Ctr Inst High Energy Phys Protvino, Protvino, Russia.
[Baines, J. T.; Barnett, B. M.; Burke, S.; Dewhurst, A.; Dopke, J.; Emeliyanov, D.; Gallop, B. J.; Gee, C. N. P.; Kirk, J.; Martin-Haugh, S.; Middleton, R. P.; Phillips, P. W.; Sankey, D. P. C.; Sawyer, C.; Tyndel, M.; Wickens, F. J.; Wielers, M.] Rutherford Appleton Lab, Particle Phys Dept, Didcot, Oxon, England.
[Anulli, F.; Bagiacchi, P.; Bagnaia, R.; Bauce, M.; Bini, C.; Ciapetti, G.; Corradi, M.; De Pedis, D.; De Salvo, A.; Di Donato, C.; Falciano, S.; Gentile, S.; Giagu, S.; Gustavino, G.; Kuna, M.; Lacava, F.; Luci, C.; Luminari, L.; Messina, A.; Nisati, A.; Pasqualucci, E.; Petrolo, E.; Pontecorvo, L.; Rescigno, M.; Rosati, S.; Tehrani, F. Safai; Vanadia, M.; Vari, R.; Veneziano, S.; Verducci, M.; Zanello, L.] Sapienza Univ Roma, Sez Roma, Ist Nazl Fis Nucl, Rome, Italy.
[Bagiacchi, P.; Bagnaia, R.; Bauce, M.; Bini, C.; Ciapetti, G.; Corradi, M.; Di Donato, C.; Gentile, S.; Giagu, S.; Gustavino, G.; Kuna, M.; Lacava, F.; Luci, C.; Messina, A.; Vanadia, M.; Verducci, M.; Zanello, L.] Sapienza Univ Roma, Dipartimento Fis, Rome, Italy.
[Aielli, G.; Camarri, P.; Cardarelli, R.; Cerrito, L.; Di Ciaccio, A.; Iuppa, R.; Liberti, B.; Salamon, A.; Santonico, R.] Univ Roma Tor Vergata, Sez Roma Tor Vergata, Ist Nazl Fis Nucl, Rome, Italy.
[Aielli, G.; Camarri, P.; Cerrito, L.; Di Ciaccio, A.; Iuppa, R.; Salamon, A.; Santonico, R.] Univ Roma Tor Vergata, Dipartimento Fis, Rome, Italy.
[Baroncelli, A.; Biglietti, M.; Ceradini, F.; Di Micco, B.; Farilla, A.; Graziani, E.; Iodice, M.; Orestano, D.; Petrucci, F.; Puddu, D.; Salamanna, G.; Sessa, M.; Stanescu, C.; Taccini, C.] Univ Roma Tre, Sez Roma Tre, Ist Nazl Fis Nucl, Rome, Italy.
[Ceradini, F.; Di Micco, B.; Orestano, D.; Petrucci, F.; Puddu, D.; Salamanna, G.; Sessa, M.; Taccini, C.] Univ Roma Tre, Dipartimento Matemat & Fis, Rome, Italy.
[Benchekroun, D.; Chafaq, A.; Hoummada] Univ Hassan 2, Reseau Univ Phys Hautes Energies, Fac Sci Ain Chock, Casablanca, Morocco.
Ctr Natl Energie Sci Tech Nucl, Rabat, Morocco.
[El Kacimi, M.; Goujdami, D.] Univ Cadi Ayyad, LPHEA Marrakech, Fac Sci Semlalia, Marrakech, Morocco.
[Aaboud, M.; Derkaoui, J. E.; Ouchrif, M.] Univ Mohamed Premier, Fac Sci, Oujda, Morocco.
[Aaboud, M.; Derkaoui, J. E.; Ouchrif, M.] LPTPM, Oujda, Morocco.
[El Moursli, R. Cherkaoui; Ezzi, M.; Fassi, F.; Haddad, N.; Idrissi, Z.; Tayalati, Y.] Univ Mohammed 5, Fac Sci, Rabat, Morocco.
[Bachacou, H.; Balli, F.; Bauer, F.; Besson, N.; Blanchard, J. -B.; Boonekamp, M.; Chevalier, L.; Hoffmann, M. Dano; Deliot, F.; Denysiuk, D.; Etienvre, A. I.; Formica, A.; Giraud, P. F.; Da Costa, J. Goncalves Pinto Firmino; Guyot, C.; Hanna, R.; Hassani, S.; Jeanneau, F.; Kivernyk, O.; Kozanecki, W.; Kukla, R.; Lancon, E.; Laporte, J. F.; Le Quilleuc, E. P.; Lesage, A. A. J.; Mansoulie, B.; Meyer, J-P.; Nicolaidou, R.; Ouraou, A.; Rodriguez, L. Pacheco; Perego, M. M.; Peyaud, A.; Saimpert, M.; Schoeffel, L.; Schune, Ph.; Schwemling, Ph.; Schwindling, J.] CEA Saclay Commissariat Energie Atom & Energies A, Inst Rech Lois Fondamentales Univers, DSM IRFU, Gif Sur Yvette, France.
[AbouZeid, O. S.; Battaglia, M.; Debenedetti, C.; Grillo, A. A.; Hance, M.; Kuhl, A.; Law, A. T.; Litke, A. M.; Lockman, W. S.; Nielsen, J.; Reece, R.; Rose, P.; Sadrozinski, H. F-W.; Schier, S.; Schumm, B. A.; Seiden, A.] Univ Calif Santa Cruz, Santa Cruz Inst Particle Phys, Santa Cruz, CA 95064 USA.
[Alpigiani, C.; Blackburn, D.; Goussiou, A. G.; Hsu, S. -C.; Johnson, W. J.; Lubatti, H. J.; Marx, M.; Meehan, S.; Rosten, R.; Rothberg, J.; Russell, H. L.; De Bruin, P. H. Sales; Pastor, E. Torro; Watts, G.] Univ Washington, Dept Phys, Seattle, WA 98195 USA.
[Anastopoulos, C.; Costanzo, D.; Donszelmann, T. Cuhadar; Dawson, I.; Fletcher, G. T.; Hamity, G. N.; Hodgkinson, M. C.; Hodgson, P.; Johansson, P.; Klinger, J. A.; Korolkova, E. V.; Kyriazopoulos, D.; Paredes, B. Lopez; Macdonald, C. M.; Miyagawa, P. S.; Parker, K. A.; Rompotis, N.; Tovey, D. R.; Vickey, T.; Boeriu, O. E. Vickey; Whallon, N. L.] Univ Sheffield, Dept Phys & Astron, Sheffield, S Yorkshire, England.
[Hasegawa, Y.; Takeshita, T.] Shinshu Univ, Dept Phys, Nagano, Japan.
[Atlay, N. B.; Buchholz, R.; Campoverde, A.; Czirr, H.; Fleck, I.; Ghasemi, S.; Ibragimov, I.; Li, Y.; Walkowiak, W.; Ziolkowski, M.] Univ Siegen, Fachbereich Phys, Siegen, Germany.
[Bnat, Q.; Horton, A. J.; Mori, D.; O'Neil, D. C.; Pachal, K.; Stelzer, B.; Temple, D.; Torres, H.; Van Nieuwkoop, J.; Vetterli, M. C.] Simon Fraser Univ, Dept Phys, Burnaby, BC, Canada.
[Armbruster, A. J.; Bawa, H. S.; Black, J. E.; Garelli, N.; Kagan, M.; Kocian, M.; Malone, C.; Moss, J.; Nachman, B. P.; Piacquadio, G.; Rubbo, F.; Salnikov, A.; Schwartzman, A.; Tompkins, L.; Wittgen, M.; Young, C.] SLAC Natl Accelerator Lab, Stanford, CA USA.
[Astalos, R.; Bartos, P.; Blazek, T.; Dado, T.; Melo, M.; Plazak, L.; Smiesko, J.; Sykora, I.; Tokar, S.; Zenis, T.] Comenius Univ, Fac Math Phys & Informat, Bratislava, Slovakia.
[Bruncko, D.; Kladiva, E.; Strizenec, P.; Urban, J.] Slovak Acad Sci, Inst Expt Phys, Dept Subnucl Phys, Kosice, Slovakia.
[Castaneda-Miranda, E.; Hamilton, A.; Yacoob, S.] Univ Cape Town, Dept Phys, Cape Town, South Africa.
[Connell, S. H.; Govender, N.] Univ Johannesburg, Dept Phys, Johannesburg, South Africa.
[Hsu, C.; Jivan, H.; Kar, D.; Garcia, B. R. Mellado; Reed, R. G.; Ruan, X.] Univ Witwatersrand, Sch Phys, Johannesburg, South Africa.
[Abulaiti, Y.; Akerstedt, H.; Asman, B.; Bendtz, K.; Bertoli, G.; Bylund, O. Bessidskaia; Bohm, C.; Clement, C.; Cribbs, W. A.; Gellerstedt, K.; Hellman, S.; Jon-And, K.; Lundberg, O.; Milstead, D. A.; Moa, T.; Molander, S.; Pani, P.; Poettgen, R.; Rossetti, V.; Shaikh, N. W.; Shcherbakova, A.; Silverstein, S. B.; Sjolin, J.; Strandberg, S.; Ughetto, M.; Santurio, E. Valdes; Wallangen, V.] Stockholm Univ, Dept Phys, Stockholm, Sweden.
[Akerstedt, H.; Asman, B.; Bendtz, K.; Bertoli, G.; Bylund, O. Bessidskaia; Clement, C.; Cribbs, W. A.; Gellerstedt, K.; Hellman, S.; Jon-And, K.; Lundberg, O.; Milstead, D. A.; Moa, T.; Molander, S.; Pani, P.; Poettgen, R.; Rossetti, V.; Shaikh, N. W.; Shcherbakova, A.; Sjolin, J.; Strandberg, S.; Ughetto, M.; Santurio, E. Valdes; Wallangen, V.] Oskar Klein Ctr, Stockholm, Sweden.
[Chen, K.; Lund-Jensen, B.; Sidebo, P. E.; Strandberg, J.; Su, D.] Royal Inst Technol, Dept Phys, Stockholm, Sweden.
[Balestri, T.; Bee, C. P.; Hobbs, J.; Huo, P.; Jia, J.; Li, H.; Lindquist, B. E.; McCarthy, R. L.; Montalbano, A.; Morvaj, L.; Radhakrishnan, S. K.; Rijssenbeek, M.; Schamberger, R. D.; Tsybychev, D.; Zaman, A.; Zhou, M.] SUNY Stony Brook, Dept Phys & Astron, Stony Brook, NY 11794 USA.
[Balestri, T.; Bee, C. P.; Hobbs, J.; Huo, P.; Jia, J.; Li, H.; Lindquist, B. E.; McCarthy, R. L.; Montalbano, A.; Morvaj, L.; Radhakrishnan, S. K.; Rijssenbeek, M.; Schamberger, R. D.; Tsybychev, D.; Zaman, A.; Zhou, M.] SUNY Stony Brook, Dept Chem, Stony Brook, NY 11794 USA.
[Abraham, N. L.; Allbrooke, B. M. M.; Asquith, L.; Cerri, A.; Barajas, C. A. Chavez; De Sanctis, U.; De Santo, A.; Lerner, G.; Miano, F.; Salvatore, F.; Castillo, I. Santoyo; Shehu, C. Y.; Suruliz, K.; Sutton, M. R.; Vivarelli, I.; Winston, O. J.] Univ Sussex, Dept Phys & Astron, Brighton, E Sussex, England.
[Black, C. W.; Finelli, K. D.; Jeng, G. -Y.; Limosani, A.; Morley, A. K.; Saavedra, A. F.; Scarcella, M.; Varvell, K. E.; Wang, J.; Yabsley, B.] Univ Sydney, Sch Phys, Sydney, NSW, Australia.
[Hou, S.; Hsu, P. J.; Lee, S. C.; Lin, S. C.; Liu, B.; Liu, D.; Lo Sterzo, F.; Mazini, R.; Shi, L.; Soh, D. A.; Teng, P. K.; Wang, S. M.; Yang, Y.] Acad Sinica, Inst Phys, Taipei, Taiwan.
[Abreu, H.; Gozani, E.; Rozen, Y.; Tarem, S.; van Eldik, N.] Technion Israel Inst Technol, Dept Phys, Haifa, Israel.
[Abramowicz, H.; Alexander, G.; Ashkenazi, A.; Bella, G.; Benary, O.; Benhammou, Y.; Davies, M.; Duarte-Campderros, J.; Etzion, E.; Gershon, A.; Gueta, O.; Oren, Y.; Soffer, A.; Taiblum, N.] Tel Aviv Univ, Raymond & Beverly Sackler Sch Phys & Astron, Tel Aviv, Israel.
[Gentsos, C.; Gkaitatzis, S.; Gkialas, I.; Iliadis, D.; Kimura, N.; Kordas, K.; Leisos, A.; Papageorgiou, K.; Petridou, C.; Sampsonidis, D.] Aristotle Univ Thessaloniki, Dept Phys, Thessaloniki, Greece.
[Adachi, S.; Asai, S.; Chen, S.; Enari, Y.; Hanawa, K.; Ishino, M.; Kanaya, N.; Kataoka, Y.; Kato, C.; Kawamoto, T.; Kishimoto, T.; Kobayashi, A.; Kobayashi, T.; Komori, Y.; Kozakai, C.; Mashimo, T.; Masubuchi, T.; Minami, Y.; Minegishi, Y.; Mori, T.; Morinaga, M.; Nakamura, T.; Ninomiya, Y.; Nobe, T.; Okumura, Y.; Saito, T.; Sakamoto, H.; Tanaka, J.; Terashi, K.; Ueda, I.; Yamamoto, S.; Yamanaka, T.] Univ Tokyo, Int Ctr Elementary Particle Phys, Tokyo, Japan.
[Adachi, S.; Asai, S.; Chen, S.; Enari, Y.; Hanawa, K.; Ishino, M.; Kanaya, N.; Kataoka, Y.; Kato, C.; Kawamoto, T.; Kishimoto, T.; Kobayashi, A.; Kobayashi, T.; Komori, Y.; Kozakai, C.; Mashimo, T.; Masubuchi, T.; Minami, Y.; Minegishi, Y.; Mori, T.; Morinaga, M.; Nakamura, T.; Ninomiya, Y.; Nobe, T.; Okumura, Y.; Saito, T.; Sakamoto, H.; Tanaka, J.; Terashi, K.; Ueda, I.; Yamamoto, S.; Yamanaka, T.] Univ Tokyo, Dept Phys, Tokyo, Japan.
[Bratzler, U.; Fukunaga, C.] Tokyo Metropolitan Univ, Grad Sch Sci & Technol, Tokyo, Japan.
[Hayakawa, D.; Ishitsuka, M.; Jinnouchi, O.; Kobayashi, D.; Kuze, M.; Motohashi, K.; Tanaka, M.; Todome, K.; Yamaguchi, D.] Tokyo Inst Technol, Dept Phys, Tokyo, Japan.
[Batista, S. J.; Chau, C. C.; Cormier, K. J. R.; DeMarco, D. A.; Di Sipio, R.; Diamond, M.; Keoshkerian, H.; Krieger, P.; Liblong, A.; Mc Goldrick, G.; Orr, R. S.; Pascuzzi, V. R.; Polifka, R.; Rudolph, M. S.; Savard, R.; Sinervo, P.; Taenzer, J.; Teuscher, R. J.; Trischuk, W.; Veloce, L. M.; Venturi, N.] Univ Toronto, Dept Phys, Toronto, ON, Canada.
[Canepa, A.; Chekulaev, S. V.; Hod, N.; Jovicevic, J.; Codina, E. Perez; Schneider, B.; Stelzer-Chilton, O.; Tafirout, R.; Trigger, I. M.] TRIUMF, Vancouver, BC, Canada.
[Ramos, J. Manjarres; Palacino, G.; Taylor, W.] York Univ, Dept Phys & Astron, Toronto, ON, Canada.
[Hagihara, M.; Hara, K.; Ito, F.; Kasahara, K.; Kim, S. H.; Kiuchi, K.; Nagata, K.; Okawa, H.; Sato, K.; Ukegawa, F.] Univ Tsukuba, Fac Pure & Appl Sci, Tsukuba, Ibaraki, Japan.
[Hagihara, M.; Hara, K.; Ito, F.; Kasahara, K.; Kim, S. H.; Kiuchi, K.; Nagata, K.; Okawa, H.; Sato, K.; Ukegawa, F.] Univ Tsukuba, Ctr Integrated Res Fundamental Sci & Engn, Tsukuba, Ibaraki, Japan.
[Beauchemin, P. H.; Meoni, E.; Sliwa, K.; Son, H.; Wetter, J.] Tufts Univ, Dept Phys & Astron, Medford, MA 02155 USA.
[Casper, D. W.; Colombo, T.; Corso-Radu, A.; Frate, M.; Guest, D.; Lankford, A. J.; Mete, A. S.; Nelson, A.; Ntekas, K.; Scannicchio, D. A.; Schernau, M.; Shimmin, C. O.; Taffard, A.; Unal, G.; Unel, G.; Whiteson, D.] Univ Calif Irvine, Dept Phys & Astron, Irvine, CA USA.
[Acharya, B. S.; Boldyrev, A. S.; Cheatham, S.; Cobal, M.; Giordani, M. P.; Pinamonti, M.; Quayle, W. B.; Serkin, L.; Shaw, K.; Soualah, R.; Truong, L.] Ist Nazl Fis Nucl, Grp Collegato Udine, Sez Trieste, Udine, Italy.
[Acharya, B. S.; Quayle, W. B.; Serkin, L.; Shaw, K.] Abdus Salaam Int Ctr Theoret Phys, Trieste, Italy.
[Boldyrev, A. S.; Cheatham, S.; Cobal, M.; Giordani, M. P.; Pinamonti, M.; Soualah, R.; Truong, L.] Univ Udine, Dipartimento Chim Fis & Ambiente, Udine, Italy.
[Brenner, R.; Ekelof, T.; Ellert, M.; Ferrari, A.; Maddocks, H. J.; Ohman, H.; Rangel-Smith, C.] Uppsala Univ, Dept Phys & Astron, Uppsala, Sweden.
[Atkinson, M.; Armadans, R. Caminal; Chang, R.; Errede, S.; Hooberman, B. H.; Khader, M.; Lie, K.; Liss, T. M.; Liu, L.; Long, J. D.; Outschoorn, V. I. Martinez; Neubauer, M. S.; Rybar, M.; Shang, R.; Sickles, A. M.; Vichou, I.; Zeng, J. C.] Univ Illinois, Dept Phys, 1110 W Green St, Urbana, IL 61801 USA.
[Alvarez Piqueras, D.; Barranco Navarro, L.; Cabrera Urban, S.; Gimenez, V. Castillo; Costa, M. J.; Fernandez Martinez, P.; Ferrer, A.; Fiorini, L.; Fuster, J.; Garcia, C.; Garcia Navarro, J. E.; Gonzalez de la Hoz, S.; Hernandez Jimenez, Y.; Higon-Rodriguez, E.; Pena, J. Jimenez; King, M.; Lacasta, C.; Lacuesta, V. R.; Mamuzic, J.; Marti-Garcia, S.; Melini, D.; Mitsou, V. A.; Lopez, S. Pedraza; Potrap, I. N.; Rodriguez, D. Rodriguez; Romero Adam, E.; Ros, E.; Salt, J.; Sanchez, J.; Sanchez Martinez, V.; Soldevila, U.; Valero, A.; Valls Ferrer, J. A.; Vos, M.] Univ Valencia, Inst Fis Corpuscular IFIC, Valencia, Spain.
[Alvarez Piqueras, D.; Barranco Navarro, L.; Cabrera Urban, S.; Gimenez, V. Castillo; Costa, M. J.; Fernandez Martinez, P.; Ferrer, A.; Fiorini, L.; Fuster, J.; Garcia, C.; Garcia Navarro, J. E.; Gonzalez de la Hoz, S.; Hernandez Jimenez, Y.; Higon-Rodriguez, E.; Pena, J. Jimenez; King, M.; Lacasta, C.; Lacuesta, V. R.; Mamuzic, J.; Marti-Garcia, S.; Melini, D.; Mitsou, V. A.; Lopez, S. Pedraza; Potrap, I. N.; Rodriguez, D. Rodriguez; Romero Adam, E.; Ros, E.; Salt, J.; Sanchez, J.; Sanchez Martinez, V.; Soldevila, U.; Valero, A.; Valls Ferrer, J. A.; Vos, M.] Univ Valencia, Dept Fis Atom Mol & Nucl, Valencia, Spain.
[Alvarez Piqueras, D.; Barranco Navarro, L.; Cabrera Urban, S.; Gimenez, V. Castillo; Costa, M. J.; Fernandez Martinez, P.; Ferrer, A.; Fiorini, L.; Fuster, J.; Garcia, C.; Garcia Navarro, J. E.; Gonzalez de la Hoz, S.; Hernandez Jimenez, Y.; Higon-Rodriguez, E.; Pena, J. Jimenez; King, M.; Lacasta, C.; Lacuesta, V. R.; Mamuzic, J.; Marti-Garcia, S.; Melini, D.; Mitsou, V. A.; Lopez, S. Pedraza; Potrap, I. N.; Rodriguez, D. Rodriguez; Romero Adam, E.; Ros, E.; Salt, J.; Sanchez, J.; Sanchez Martinez, V.; Soldevila, U.; Valero, A.; Valls Ferrer, J. A.; Vos, M.] Univ Valencia, Dept Ingn Elect, Valencia, Spain.
[Alvarez Piqueras, D.; Barranco Navarro, L.; Cabrera Urban, S.; Gimenez, V. Castillo; Costa, M. J.; Fernandez Martinez, P.; Ferrer, A.; Fiorini, L.; Fuster, J.; Garcia, C.; Garcia Navarro, J. E.; Gonzalez de la Hoz, S.; Higon-Rodriguez, E.; Pena, J. Jimenez; King, M.; Lacasta, C.; Lacuesta, V. R.; Mamuzic, J.; Marti-Garcia, S.; Melini, D.; Mitsou, V. A.; Lopez, S. Pedraza; Potrap, I. N.; Rodriguez, D. Rodriguez; Romero Adam, E.; Ros, E.; Salt, J.; Sanchez, J.; Sanchez Martinez, V.; Soldevila, U.; Valero, A.; Valls Ferrer, J. A.; Vos, M.] Univ Valencia, Inst Microelect Barcelona IMB CNM, Valencia, Spain.
[Alvarez Piqueras, D.; Barranco Navarro, L.; Biebel, O.; Cabrera Urban, S.; Gimenez, V. Castillo; Costa, M. J.; Fernandez Martinez, P.; Ferrer, A.; Fiorini, L.; Fuster, J.; Garcia, C.; Garcia Navarro, J. E.; Gonzalez de la Hoz, S.; Hernandez Jimenez, Y.; Higon-Rodriguez, E.; Pena, J. Jimenez; King, M.; Lacasta, C.; Lacuesta, V. R.; Mamuzic, J.; Marti-Garcia, S.; Melini, D.; Mitsou, V. A.; Lopez, S. Pedraza; Potrap, I. N.; Rodriguez, D. Rodriguez; Romero Adam, E.; Ros, E.; Salt, J.; Sanchez, J.; Sanchez Martinez, V.; Soldevila, U.; Valero, A.; Valls Ferrer, J. A.; Vos, M.] CSIC, Valencia, Spain.
[Kuutmann, E. Bergeaas; Danninger, M.; Fedorko, W.; Gay, C.; Gecse, Z.; Gignac, M.; Henkelmann, S.; Lister, A.] Univ British Columbia, Dept Phys, Vancouver, BC, Canada.
[Albert, J.; David, C.; Elliot, A. A.; Fincke-Keeler, M.; Hamano, K.; Hill, E.; Keeler, R.; Kowalewski, R.; Kuwertz, E. S.; LeBlanc, M.; Lefebvre, M.; McPherson, R. A.; Pearce, J.; Seuster, R.; Sobie, R.; Trovatelli, M.; Venturi, M.] Univ Victoria, Dept Phys & Astron, Victoria, BC, Canada.
[Beckingham, M.; Ennis, J. S.; Farrington, S. M.; Harrison, P. F.; Jeske, C.; Jones, G.; Martin, T. A.; Murray, W. J.; Pianori, E.; Spangenberg, M.] Univ Warwick, Dept Phys, Coventry, W Midlands, England.
[Iizawa, T.; Kaji, T.; Mitani, T.; Sakurai, Y.; Yorita, K.] Waseda Univ, Tokyo, Japan.
[Balek, R.; Bressler, S.; Citron, Z. H.; Duchovni, E.; Dumancic, M.; Gross, E.; Kohler, M. K.; Lellouch, D.; Levinson, L. J.; Mikenberg, G.; Milov, A.; Pitt, M.; Ravinovich, I.; Roth, I.; Schaarschmidt, J.; Smakhtin, V.; Turgeman, D.] Weizmann Inst Sci, Dept Particle Phys, Rehovot, Israel.
[Banerjee, Sw.; Biebel, O.; Guan, W.; Hard, A. S.; Heng, Y.; Ji, H.; Ju, X.; Kaplan, L. S.; Kashif, L.; Ming, Y.; Wang, F.; Wiedenmann, W.; Wu, S. L.; Yang, H.; Zhang, F.; Zhou, C.; Zobernig, G.] Univ Wisconsin, Dept Phys, 1150 Univ Ave, Madison, WI 53706 USA.
[Herget, V.; Kuger, F.; Redelbach, A.; Schreyer, M.; Sidiropoulou, O.; Siragusa, G.; Stroehmer, R.; Trefzger, T.; Weber, S. W.; Zibell, A.] Julius Maximilians Univ, Fak Phys & Astron, Wurzburg, Germany.
[Bannoura, A. A. E.; Boerner, D.; Cornelissen, T.; Ellinghaus, F.; Ernis, G.; Fischer, J.; Flick, T.; Gabizon, O.; Gilles, G.; Hamacher, K.; Hirschbuehl, D.; Kersten, S.; Kuechler, J. T.; Maettig, P.; Neumann, M.; Pataraia, S.; Riegel, C. J.; Sandhoff, M.; Tepel, F.; Vogel, M.; Zeitnitz, C.] Berg Univ Wuppertal, Fak Math & Nat Wissensch, Fachgrp Phys, Wuppertal, Germany.
[Baker, O. K.; Noccioli, E. Benhar; Cummings, J.; Demers, S.; Ideal, E.; Lagouri, T.; Leister, A. G.; Loginov, A.; Paganini, M.; Hernandez, D. Paredes; Thomsen, L. A.; Tipton, P.; Vasquez, J. G.; Wang, X.] Yale Univ, Dept Phys, New Haven, CT USA.
[Hakobyan, H.; Vardanyan, G.] Yerevan Phys Inst, Yerevan, Armenia.
[Rahal, G.] IN2P3, Ctr Calcul, Villeurbanne, France.
[Acharya, B. S.] Kings Coll London, Dept Phys, London, England.
[Ahmadov, F.; Huseynov, N.; Javadov, N.] Azerbaijan Acad Sci, Inst Phys, Baku, Azerbaijan.
[Anisenkov, A. V.; Baldin, E. M.; Bobrovnikov, V. S.; Buzykaev, A. R.; Kazanin, V. F.; Kharlamov, A. G.; Korol, A. A.; Maslennikov, A. L.; Maximov, D. A.; Peleganchuk, S. V.; Rezanova, O. L.; Soukharev, A. M.; Talyshev, A. A.; Tikhonov, Yu. A.] Novosibirsk State Univ, Novosibirsk, Russia.
[Azuelos, G.; Gingrich, D. M.; Oakham, F. G.; Savard, R.; Vetterli, M. C.] TRIUMF, Vancouver, BC, Canada.
[Banerjee, Sw.] Univ Louisville, Dept Phys & Astron, Louisville, KY 40292 USA.
[Bawa, H. S.; Gao, Y. S.] Calif State Univ Fresno, Dept Phys, Fresno, CA 93740 USA.
[Beck, H. P.] Univ Fribourg, Dept Phys, Fribourg, Switzerland.
[Casado, M. P.] Univ Autonoma Barcelona, Dept Fis, Barcelona, Spain.
[Castro, N. F.] Univ Porto, Dept Fis & Astron, Fac Ciencias, Oporto, Portugal.
[Chelkov, G. A.] Tomsk State Univ, Tomsk, Russia.
[Conventi, F.; Della Pietra, M.] Univ Napoli Parthenope, Naples, Italy.
[Corriveau, F.; McPherson, R. A.; Robertson, S. H.; Sobie, R.; Teuscher, R. J.] Inst Particle Phys IPP, Ottawa, ON, Canada.
[Ducu, O. A.] Natl Inst Phys & Nucl Engn, Bucharest, Romania.
[Fedin, O. L.] St Petersburg State Polytech Univ, Dept Phys, St Petersburg, Russia.
[Geng, C.; Guo, Y.; Li, B.] Univ Michigan, Dept Phys, Ann Arbor, MI 48109 USA.
[Govender, N.] Ctr High Performance Comp, CSIR Campus, Cape Town, South Africa.
[Greenwood, Z. D.; Sawyer, L.] Louisiana Tech Univ, Ruston, LA 71270 USA.
[Grinstein, S.; Rozas, A. Juste; Martinez, M.] ICREA, Barcelona, Spain.
[Hanagaki, K.] Osaka Univ, Grad Sch Sci, Osaka, Japan.
[Hsu, P. J.] Natl Tsing Hua Univ, Dept Phys, Taipei, Taiwan.
[Igonkina, O.] Radboud Univ Nijmegen Nikhef, Inst Math Astrophys & Particle Phys, Nijmegen, Netherlands.
[Ilchenko, Y.; Onyisi, P. U. E.] Univ Texas Austin, Dept Phys, Austin, TX 78712 USA.
[Jenni, P.] CERN, Geneva, Switzerland.
[Khubua, J.] Georgian Tech Univ GTU, Tbilisi, Rep of Georgia.
[Kono, T.; Nagai, R.] Ochanomizu Univ, Ochadai Acad Prod, Tokyo, Japan.
[Konoplich, R.] Manhattan Coll, New York, NY USA.
[Leisos, A.] Hellen Open Univ, Patras, Greece.
[Lin, S. C.] Acad Sinica, Acad Sinica Grid Comp, Inst Phys, Taipei, Taiwan.
[Liu, B.] Shandong Univ, Sch Phys, Jinan, Shandong, Peoples R China.
[Myagkov, A. G.; Nikolaenko, V.; Zaitsev, A. M.] State Univ, Moscow Inst Phys & Technol, Dolgoprudnyi, Russia.
[Nessi, M.] Univ Geneva, Sect Phys, Geneva, Switzerland.
[Pasztor, G.] Eotvos Lorand Univ, Budapest, Hungary.
[Piacquadio, G.] SUNY Stony Brook, Dept Phys & Astron, Stony Brook, NY 11794 USA.
[Piacquadio, G.] SUNY Stony Brook, Dept Chem, Stony Brook, NY 11794 USA.
[Pinamonti, M.] Int Sch Adv Studies SISSA, Trieste, Italy.
[Purohit, M.] Univ S Carolina, Dept Phys & Astron, Columbia, SC 29208 USA.
[Shi, L.] Sun Yat Sen Univ, Sch Phys & Engn, Guangzhou, Guangdong, Peoples R China.
[Shiyakova, M.] Bulgarian Acad Sci, Inst Nucl Res & Nucl Energy INRNE, Sofia, Bulgaria.
[Smirnova, L. N.] Moscow MV Lomonosov State Univ, Fac Phys, Moscow, Russia.
[Song, H. Y.; Zhang, G.] Acad Sinica, Inst Phys, Taipei, Taiwan.
[Tikhomirov, V. O.] Natl Res Nucl Univ MEPhI, Moscow, Russia.
[Tompkins, L.] Stanford Univ, Dept Phys, Stanford, CA 94305 USA.
[Toth, J.] Wigner Res Ctr Phys, Inst Particle & Nucl Phys, Budapest, Hungary.
[Vest, A.] Flensburg Univ Appl Sci, Flensburg, Germany.
[Yusuff, I.] Univ Malaya, Dept Phys, Kuala Lumpur, Malaysia.
[Zhang, R.] Aix Marseille Univ, CPPM, Aix En Provence, France.
[Zhang, R.] CNRS IN2P3, Marseille, France.
PKU CHEP, Beijing, Peoples R China.
RP Aaboud, M (reprint author), Univ Mohamed Premier, Fac Sci, Oujda, Morocco.; Aaboud, M (reprint author), LPTPM, Oujda, Morocco.
RI Kuday, Sinan/C-8528-2014; Soldatov, Evgeny/E-3990-2017; Doyle,
Anthony/C-5889-2009; Mitsou, Vasiliki/D-1967-2009; Garcia, Jose
/H-6339-2015; Solodkov, Alexander/B-8623-2017; Camarri,
Paolo/M-7979-2015; Carvalho, Joao/M-4060-2013; Prokoshin,
Fedor/E-2795-2012; Guo, Jun/O-5202-2015; Livan, Michele/D-7531-2012;
Gladilin, Leonid/B-5226-2011; Villa, Mauro/C-9883-2009; Peleganchuk,
Sergey/J-6722-2014; messina, andrea/C-2753-2013; Yang,
Haijun/O-1055-2015; White, Ryan/E-2979-2015; Li, Liang/O-1107-2015;
Monzani, Simone/D-6328-2017; Warburton, Andreas/N-8028-2013; Tikhomirov,
Vladimir/M-6194-2015
OI Kuday, Sinan/0000-0002-0116-5494; Soldatov, Evgeny/0000-0003-0694-3272;
Doyle, Anthony/0000-0001-6322-6195; Mitsou,
Vasiliki/0000-0002-1533-8886; Solodkov, Alexander/0000-0002-2737-8674;
Camarri, Paolo/0000-0002-5732-5645; Carvalho, Joao/0000-0002-3015-7821;
Prokoshin, Fedor/0000-0001-6389-5399; Veneziano,
Stefano/0000-0002-2598-2659; Belanger-Champagne,
Camille/0000-0003-2368-2617; Belyaev, Nikita/0000-0002-1131-7121; Guo,
Jun/0000-0001-8125-9433; Livan, Michele/0000-0002-5877-0062; Gladilin,
Leonid/0000-0001-9422-8636; Villa, Mauro/0000-0002-9181-8048;
Peleganchuk, Sergey/0000-0003-0907-7592; White,
Ryan/0000-0003-3589-5900; Li, Liang/0000-0001-6411-6107; Monzani,
Simone/0000-0002-0479-2207; Warburton, Andreas/0000-0002-2298-7315;
Tikhomirov, Vladimir/0000-0002-9634-0581
FU ANPCyT, Argentina; YerPhI, Armenia; ARC, Australia; BMWFW, Austria; FWF,
Austria; ANAS, Azerbaijan; SSTC, Belarus; CNPq, Brazil; FAPESP, Brazil;
NSERC, Canada; NRC, Canada; CFI, Canada; CERN; CONICYT, Chile; CAS,
China; MOST, China; NSFC, China; COLCIENCIAS, Colombia; MSMT CR, Czech
Republic; MPO CR, Czech Republic; VSC CR, Czech Republic; DNRF, Denmark;
DNSRC, Denmark; IN2P3-CNRS, CEA-DSM/IRFU, France; GNSF, Georgia; BMBF,
Germany; HGF, Germany; MPG, Germany; GSRT, Greece; RGC, Hong Kong SAR,
China; ISF, Israel; I-CORE, Israel; Benoziyo Center, Israel; INFN,
Italy; MEXT, Japan; JSPS, Japan; CNRST, Morocco; FOM, Netherlands; NWO,
Netherlands; RCN, Norway; MNiSW, Poland; NCN, Poland; FCT, Portugal;
MNE/IFA, Romania; MES of Russia, Russian Federation; NRC KI, Russian
Federation; JINR; MESTD, Serbia; MSSR, Slovakia; ARRS, Slovenia; MIZS,
Slovenia; DST/NRF, South Africa; MINECO, Spain; SRC, Sweden; Wallenberg
Foundation, Sweden; SERI, Switzerland; SNSF, Switzerland; Canton of
Bern, Switzerland; Canton of Geneva, Switzerland; MOST, Taiwan; TAEK,
Turkey; STFC, United Kingdom; DOE, United States of America; NSF, United
States of America; BCKDF, Canada; Canada Council, Canada; Canarie,
Canada; CRC, Canada; Compute Canada, Canada; FQRNT, Canada; Ontario
Innovation Trust, Canada; EPLANET, European Union; ERC, European Union;
FP7, European Union; Horizon, European Union; Marie Sklodowska-Curie
Actions, European Union; Investissement d'Avenir Labex, France;
Investissements d'Avenir Idex, France; ANR, France; Region Auvergne,
France; Fondation Partager le Savoir, France; DFG, Germany; AvH
Foundation, Germany; Herakleitos programme; Thales programme; Aristeia
programme - EU-ESF; Greek NSRF; BSF, Israel; GIF, Israel; Minerva,
Israel; BRF, Norway; Generalitat de Catalunya, Generalitat Valenciana,
Spain; Royal Society, United Kingdom; Leverhulme Trust, United Kingdom
FX We acknowledge the support of ANPCyT, Argentina; YerPhI, Armenia; ARC,
Australia; BMWFW and FWF, Austria; ANAS, Azerbaijan; SSTC, Belarus; CNPq
and FAPESP, Brazil; NSERC, NRC and CFI, Canada; CERN; CONICYT, Chile;
CAS, MOST and NSFC, China; COLCIENCIAS, Colombia; MSMT CR, MPO CR and
VSC CR, Czech Republic; DNRF and DNSRC, Denmark; IN2P3-CNRS,
CEA-DSM/IRFU, France; GNSF, Georgia; BMBF, HGF, and MPG, Germany; GSRT,
Greece; RGC, Hong Kong SAR, China; ISF, I-CORE and Benoziyo Center,
Israel; INFN, Italy; MEXT and JSPS, Japan; CNRST, Morocco; FOM and NWO,
Netherlands; RCN, Norway; MNiSW and NCN, Poland; FCT, Portugal; MNE/IFA,
Romania; MES of Russia and NRC KI, Russian Federation; JINR; MESTD,
Serbia; MSSR, Slovakia; ARRS and MIZS, Slovenia; DST/NRF, South Africa;
MINECO, Spain; SRC and Wallenberg Foundation, Sweden; SERI, SNSF and
Cantons of Bern and Geneva, Switzerland; MOST, Taiwan; TAEK, Turkey;
STFC, United Kingdom; DOE and NSF, United States of America. In
addition, individual groups and members have received support from
BCKDF, the Canada Council, Canarie, CRC, Compute Canada, FQRNT, and the
Ontario Innovation Trust, Canada; EPLANET, ERC, FP7, Horizon 2020 and
Marie Sklodowska-Curie Actions, European Union; Investissements d'Avenir
Labex and Idex, ANR, Region Auvergne and Fondation Partager le Savoir,
France; DFG and AvH Foundation, Germany; Herakleitos, Thales and
Aristeia programmes co-financed by EU-ESF and the Greek NSRF; BSF, GIF
and Minerva, Israel; BRF, Norway; Generalitat de Catalunya, Generalitat
Valenciana, Spain; the Royal Society and Leverhulme Trust, United
Kingdom.
NR 51
TC 0
Z9 0
U1 26
U2 26
PU ELSEVIER SCIENCE BV
PI AMSTERDAM
PA PO BOX 211, 1000 AE AMSTERDAM, NETHERLANDS
SN 0370-2693
EI 1873-2445
J9 PHYS LETT B
JI Phys. Lett. B
PD OCT 10
PY 2016
VL 761
BP 158
EP 178
DI 10.1016/j.physletb.2016.08.020
PG 21
WC Astronomy & Astrophysics; Physics, Nuclear; Physics, Particles & Fields
SC Astronomy & Astrophysics; Physics
GA DX6CI
UT WOS:000384469900024
ER
PT J
AU Aaboud, M
Aad, G
Abbott, B
Abdallah, J
Abdinov, O
Abeloos, B
Aben, R
AbouZeid, OS
Abraham, NL
Abramowicz, H
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Abulaiti, Y
Acharya, BS
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Yu, D. R.
Yu, J.
Yu, J. M.
Yu, J.
Yuan, L.
Yuen, S. P. Y.
Yusuff, I.
Zabinski, B.
Zaidan, R.
Zaitsev, A. M.
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Zhao, Z.
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Zhu, C. G.
Zhu, H.
Zhu, J.
Zhu, Y.
Zhuang, X.
Zhukov, K.
Zibell, A.
Zieminska, D.
Zimine, N. I.
Zimmermann, C.
Zimmermann, S.
Zinonos, Z.
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Ziolkowski, M.
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Zwalinski, L.
CA ATLAS Collaboration
TI Measurement of the top quark mass in the t(t)over-bar -> dilepton
channel from root s=8TeVATLAS data
SO PHYSICS LETTERS B
LA English
DT Article
ID PARTON DISTRIBUTIONS; HADRON COLLIDERS; STANDARD MODEL; PLUS PLUS; LHC;
FRAGMENTATION; PHYSICS
AB The top quark mass is measured in the t (t) over bar -> dilepton channel (lepton= e, mu) using ATLAS data recorded in the year 2012 at the LHC. The data were taken at a proton-proton centre-of-mass energy of root s = 8 TeV and correspond to an integrated luminosity of about 20.2 fb(-1). Exploiting the template method, and using the distribution of invariant masses of lepton-b-jetpairs, the top quark mass is measured to be m(top) = 172.99 +/- 0.41(stat)+/- 0.74(syst) GeV, with a total uncertainty of 0.84 GeV. Finally, acombination with previous ATLAS m(top) measurements from root s = 7 TeV data in the t (t) over bar -> dilepton and t (t) over bar -> lepton + jets channels results in m(top) = 172.84 +/- 0.34(stat)+/- 0.61(syst) GeV, with a total uncertainty of 0.70 GeV. (C) 2016 The Author. Published by Elsevier B.V.
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[Bouffard, J.; Ernst, J.; Fischer, A.; Guindon, S.; Jain, V.] SUNY Albany, Dept Phys, Albany, NY 12222 USA.
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[Cakir, O.; Ciftci, A. K.; Yildiz, H. Duran] Ankara Univ, Dept Phys, Ankara, Turkey.
[Kuday, S.] Istanbul Aydin Univ, Istanbul, Turkey.
[Sultansoy, S.] TOBB Univ Econ & Technol, Div Phys, Ankara, Turkey.
[Barnovska, Z.; Berger, N.; Delmastro, M.; Di Ciaccio, L.; Elles, S.; Grevtsov, K.; Guillemin, T.; Hryn'ova, T.; Jezequel, S.; Koletsou, I.; Lafaye, R.; Leveque, J.; Mastrandrea, P.; Sauvage, G.; Sauvan, E.; Smart, B. H.; Todorov, T.; Wingerter-Seez, I.; Yatsenko, E.] CNRS, IN2P3, LAPP, Annecy Le Vieux, France.
[Barnovska, Z.; Berger, N.; Delmastro, M.; Di Ciaccio, L.; Elles, S.; Grevtsov, K.; Guillemin, T.; Hryn'ova, T.; Jezequel, S.; Koletsou, I.; Lafaye, R.; Leveque, J.; Mastrandrea, P.; Sauvage, G.; Sauvan, E.; Smart, B. H.; Todorov, T.; Wingerter-Seez, I.; Yatsenko, E.] Univ Savoie Mont Blanc, Annecy Le Vieux, France.
[Blair, R. E.; Chekanov, S.; LeCompte, T.; Love, J.; Malon, D.; Metcalfe, J.; Nguyen, D. H.; Paramonov, A.; Price, L. E.; Proudfoot, J.; Ryu, S.; Stanek, R. W.; van Gemmeren, P.; Wang, R.; Webster, J. S.; Yoshida, R.; Zhang, J.] Argonne Natl Lab, Div High Energy Phys, Argonne, IL 60439 USA.
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[Alexopoulos, T.; Benekos, N.; Dris, M.; Gazis, E. N.; Karakostas, K.; Karastathis, N.; Karentzos, E.; Leontsinis, S.; Maltezos, S.; Ntekas, K.; St Panagiotopoulou, E.; Papadopoulou, Th. D.; Tsipolitis, G.; Vlachos, S.] Natl Tech Univ Athens, Dept Phys, Zografos, Greece.
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[Arslan, O.; Bechtle, P.; Bernlochner, F. U.; Brock, I.; Bruscino, N.; Caudron, J.; Cioara, I. A.; Cristinziani, M.; Davey, W.; Desch, K.; Dingfelder, J.; Gaycken, G.; Geich-Gimbel, Ch.; Ghneimat, M.; Grefe, C.; Hagebock, S.; Hansen, M. C.; Hohn, D.; Huegging, F.; Janssen, J.; Kostyukhin, V. V.; Kroseberg, J.; Kruger, H.; Lantzsch, K.; Lenz, T.; Leyko, A. M.; Liebal, J.; Moles-Valls, R.; Obermann, T.; Pohl, D.; Ricken, O.; Sarrazin, B.; Schaepe, S.; Schopf, E.; Schultens, M. J.; Schwindt, T.; Seema, P.; Stillings, J. A.; von Toerne, E.; Wagner, P.; Wang, T.; Wermes, N.; Wienemann, P.; Wiik-Fuchs, L. A. M.; Winter, B. T.; Wong, K. H. Yau; Yuen, S. P. Y.; Zhang, R.] Univ Bonn, Inst Phys, Bonn, Germany.
[Ahlen, S. P.; Black, K. M.; Butler, J. M.; Dell'Asta, L.; Kruskal, M.; Long, B. A.; Shank, J. T.; Yan, Z.; Youssef, S.] Boston Univ, Dept Phys, 590 Commonwealth Ave, Boston, MA 02215 USA.
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[Coutinho, Y. Amaral; Caloba, L. P.; Maidantchik, C.; Marroquim, F.; Nepomuceno, A. A.; Seixas, J. M.] Univ Fed Rio de Janeiro, COPPE, EE, IF, Rio De Janeiro, Brazil.
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Transilvania Univ Brasov, Brasov, Romania.
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[Popeneciu, G. A.] Natl Inst Res & Dev Isotop & Mol Technol, Dept Phys, Cluj Napoca, Romania.
Univ Politehn Bucuresti, Bucharest, Romania.
[Gravila, P. M.] West Univ Timisoara, Timisoara, Romania.
[Sola, J. D. Bossio; Marceca, G.; Otero Y Garzon, G.; Piegaia, R.; Reisin, H.; Sacerdoti, S.] Univ Buenos Aires, Dept Fis, Buenos Aires, DF, Argentina.
[Arratia, M.; Barlow, N.; Batley, J. R.; Brochu, F. M.; Brunt, B. H.; Carter, J. R.; Chapman, J. D.; Cottin, G.; Gillam, T. P. S.; Hill, J. C.; Kaneti, S.; Lester, C. G.; Mueller, T.; Parker, M. A.; Potter, C. J.; Robinson, D.; Rosten, J. H. N.; Thomson, M.; Ward, C. P.; Yusuff, I.] Univ Cambridge, Cavendish Lab, Cambridge, England.
[Bellerive, A.; Cree, G.; Di Valentino, D.; Gillberg, D.; Koffas, T.; Lacey, J.; Leight, W. A.; Nomidis, I.; Oakham, F. G.; Pasztor, G.; Ruiz-Martinez, A.; Vincter, M. G.] Carleton Univ, Dept Phys, Ottawa, ON, Canada.
[Aleksa, M.; Alvarez Gonzalez, B.; Amoroso, S.; Anders, G.; Anghinolfi, F.; Arnaez, O.; Avolio, G.; Baak, M. A.; Backhaus, M.; Barak, L.; Barisits, M-S; Beermann, T. A.; Beltramello, O.; Bianco, M.; Bogaerts, J. A.; Bortfeldt, J.; Boveia, A.; Boyd, J.; Burckhart, H.; Camarda, S.; Campana, S.; Garrido, M. D. M. Capeans; Carli, T.; Carrillo-Montoya, G. D.; Catinaccio, A.; Cattai, A.; Cerv, M.; Chromek-Burckhart, D.; Colombo, T.; Conti, G.; Cortes-Gonzalez, A.; Dell'Acqua, A.; Deviveiros, P. O.; Di Girolamo, A.; Di Girolamo, B.; Di Nardo, R.; Dimitrievska, A.; Dittus, F.; Dobos, D.; Dudarev, A.; Duhrssen, M.; Eifert, T.; Ellis, N.; Elsing, M.; Farthouat, P.; Fassnacht, P.; Feng, E. J.; Francis, D.; Fressard-Batraneanu, S. M.; Froidevaux, D.; Gadatsch, S.; Glatzer, J.; Goossens, L.; Gorini, B.; Gray, H. M.; Gumpert, C.; Hanisch, S.; Hawkings, R. J.; Helary, L.; Helsens, C.; Correia, A. M. Henriques; Hervas, L.; Hoecker, A.; Huhtinen, M.; Lengo, P.; Jakobsen, S.; Klioutchnikova, T.; Krasznahorkay, A.; Lapoire, C.; Lassnig, M.; Miotto, G. Lehmann; Lenzi, B.; Lichard, P.; Malyukov, S.; Mandelli, B.; Manousos, A.; Mapelli, L.; Marzin, A.; Berlingen, J. Montejo; Mornacchi, G.; Nairz, A. M.; Nessi, M.; Nordberg, M.; Oide, H.; Palestini, S.; Pauly, T.; Pernegger, H.; Petersen, B. A.; Pommes, K.; Poppleton, A.; Poulard, G.; Poveda, J.; Astigarraga, M. E. Pozo; Rammensee, M.; Raymond, M.; Rembser, C.; Ritsch, E.; Roe, S.; Ruthmann, N.; Salzburger, A.; Schaefer, D.; Schlenker, S.; Schmieden, K.; Sforza, F.; Sanchez, C. A. Solans; Spigo, G.; Starz, S.; Stelzer, H. J.; Teischinger, F. A.; Ten Kate, H.; Unal, G.; van Woerden, M. C.; Vandelli, W.; Ventura, A.; Voss, R.; Vuillermet, R.; Wells, P. S.; Wengler, T.; Wenig, S.; Werner, P.; Wilkens, H. G.; Wotschack, J.; Young, C. J. S.; Zwalinski, L.] CERN, Geneva, Switzerland.
[Alison, J.; Anderson, K. J.; Bryant, P.; Toro, R. Camacho; Cheng, Y.; Dandoy, J. R.; Facini, G.; Gardner, R. W.; Kapliy, A.; Kim, Y. K.; Krizka, K.; Li, H. L.; Merritt, F. S.; Miller, D. W.; Oreglia, M. J.; Pilcher, J. E.; Saxon, J.; Shochet, M. J.; Stark, G. H.; Swiatlowski, M.; Vukotic, I.; Wu, M.] Univ Chicago, Enrico Fermi Inst, 5640 S Ellis Ave, Chicago, IL 60637 USA.
[Blunier, S.; Diaz, M. A.; Ochoa-Ricoux, J. P.] Pontificia Univ Catolica Chile, Dept Fis, Santiago, Chile.
[Brooks, W. K.; Carquin, E.; Kuleshov, S.; Pezoa, R.; Prokoshin, F.; Loyola, J. E. Salazar; Araya, S. Tapia; White, R.] Univ Tecn Federico Santa Maria, Dept Fis, Valparaiso, Chile.
[Bai, Y.; Barreiro Guimaraes da Costa, J.; Cheng, H. J.; Fang, Y.; Jin, S.; Li, Q.; Liang, Z.; Merino, J. Llorente; Lou, X.; Mansour, J. D.; Ouyang, Q.; Peng, C.; Ren, H.; Shan, L. Y.; Sun, X.; Xu, D.; Zhu, H.; Zhuang, X.] Chinese Acad Sci, Inst High Energy Phys, Beijing, Peoples R China.
[Gao, J.; Geng, C.; Guo, Y.; Han, L.; Hu, Q.; Jiang, Y.; Li, B.; Li, C.; Liu, J. B.; Liu, M.; Liu, Y. L.; Liu, Y.; Peng, H.; Sood, A.; Wang, W.; Zhang, G.; Zhang, R.; Zhao, Z.; Zhu, Y.] Univ Sci & Technol China, Dept Modern Phys, Hefei, Anhui, Peoples R China.
[Chen, S.; Wang, C.; Zhang, H.] Nanjing Univ, Dept Phys, Nanjing, Jiangsu, Peoples R China.
[Du, Y.; Feng, C.; Ma, L. L.; Ma, Y.; Wang, C.; Zaidan, R.; Zhang, X.; Zhao, Y.; Zhu, C. G.] Shandong Univ, Sch Phys, Jinan, Shandong, Peoples R China.
[Bret, M. Cano; Guo, J.; Hu, S.; Li, L.; Yang, H.] Shanghai Jiao Tong Univ, Shanghai Key Lab Particle Phys & Cosmol, Dept Phys & Astron, Shanghai, Peoples R China.
[Chen, X.; Zhou, N.] Tsinghua Univ, Dept Phys, Beijing 100084, Peoples R China.
[Boumediene, D.; Busato, E.; Calvet, D.; Calvet, S.; Chomont, A. R.; Donini, J.; Gris, Ph.; Madar, R.; Pallin, D.; Saez, S. M. Romano; Santoni, C.; Simon, D.; Vazeille, F.] Clermont Univ, Phys Corpusculaire Lab, Clermont Ferrand, France.
[Alkire, S. P.; Angerami, A.; Brooijmans, G.; Carbone, R. M.; Clark, M. R.; Cole, B.; Hu, D.; Hughes, E. W.; Iordanidou, K.; Klein, M. H.; Mohapatra, S.; Ochoa, I.; Persons, J. A.; Smith, M. N. K.; Smith, R. W.; Thompson, E. N.; Tuts, P. M.; Wang, T.; Zhou, L.] Columbia Univ, Nevis Lab, Irvington, NY USA.
[Alonso, A.; Besjes, G. J.; Dam, M.; Galster, G.; Hansen, J. B.; Hansen, J. D.; Hansen, P. H.; Loevschall-Jensen, A. E.; Monk, J.; Mortensen, S. S.; Pedersen, L. E.; Petersen, T. C.; Pingel, A.; Policicchio, A.; Wiglesworth, C.; Xella, S.] Univ Copenhagen, Niels Bohr Inst, Copenhagen, Denmark.
[Cairo, V. M.; Callea, G.; Capua, M.; Crosetti, G.; Del Gaudio, M.; La Rotonda, L.; Mastroberardino, A.; Policicchio, A.; Salvatore, D.; Scarfone, V.; Schioppa, M.; Susinno, G.; Tassi, E.] INFN Grp Collegato Cosenza, Lab Nazl Frascati, Frascati, Italy.
[Cairo, V. M.; Callea, G.; Capua, M.; Crosetti, G.; Del Gaudio, M.; La Rotonda, L.; Mastroberardino, A.; Salvatore, D.; Scarfone, V.; Schioppa, M.; Susinno, G.; Tassi, E.] Univ Calabria, Dipartimento Fis, Arcavacata Di Rende, Italy.
[Adamczyk, L.; Bold, T.; Dabrowski, W.; Gach, G. P.; Grabowska-Bold, I.; Kisielewska, D.; Koperny, S.; Kowalski, T. Z.; Mindur, B.; Przybycien, M.; Zemla, A.] AGH Univ Sci & Technol, Fac Phys & Appl Comp Sci, Krakow, Poland.
[Palka, M.; Richter-Was, E.] Jagiellonian Univ, Marian Smoluchowski Inst Phys, Krakow, Poland.
[Banas, E.; de Renstrom, P. A. Bruckman; Burka, K.; Chwastowski, J. J.; Derendarz, D.; Godlewski, J.; Gornicki, E.; Hajduk, Z.; Iwanski, W.; Kaczmarska, A.; Knapik, J.; Korcyl, K.; Kowalewska, A. B.; Malecki, Pa.; Olszewski, A.; Olszowska, J.; Stanecka, E.; Staszewski, R.; Trzebinski, M.; Trzupek, A.; Wolter, M. W.; Wosiek, B. K.; Wozniak, K. W.; Zabinski, B.] Polish Acad Sci, Inst Nucl Phys, Krakow, Poland.
[Cao, T.; Firan, A.; Gupta, R.; Hetherly, J. W.; Kama, S.; Kehoe, R.; Sekula, S. J.; Stroynowski, R.; Turvey, A. J.; Varol, T.; Wang, H.; Ye, J.; Zhao, X.; Zhou, L.] Southern Methodist Univ, Dept Phys, Dallas, TX USA.
[Izen, J. M.; Leyton, M.; Meirose, B.; Namasivayam, H.; Reeves, K.] Univ Texas Dallas, Dept Phys, Richardson, TX USA.
[Asbah, N.; Behr, J. K.; Bertsche, C.; Bessner, M.; Bloch, I.; Britzger, D.; Deterre, C.; Dutta, B.; Dyndal, M.; Eckardt, C.; Filipuzzi, M.; Flaschel, N.; Bravo, A. Gascon; Gasnikova, K.; Glazov, A.; Gregor, I. M.; Haleem, M.; Hamnett, P. G.; Hiller, K. H.; Howarth, J.; Huang, Y.; Katzy, J.; Keller, J. S.; Kondrashova, N.; Kuhl, T.; Lobodzinska, E.; Lohwasser, K.; Madsen, A.; Medinnis, M.; Monig, K.; Garcia, R. F. Naranjo; Naumann, T.; O'Rourke, A. A.; Peschke, R.; Peters, K.; Pirumov, H.; Poley, A.; Robinson, J. E. M.; Schaefer, R.; Schmitt, S.; South, D.; Stanescu-Bellu, M.; Stanitzki, M. M.; Styles, N. A.; Tackmann, K.; Trofymov, A.; Wang, J.; Zakharchuk, N.] DESY, Hamburg, Germany.
[Asbah, N.; Behr, J. K.; Bertsche, C.; Bessner, M.; Bloch, I.; Britzger, D.; Deterre, C.; Dutta, B.; Dyndal, M.; Eckardt, C.; Filipuzzi, M.; Flaschel, N.; Bravo, A. Gascon; Gasnikova, K.; Glazov, A.; Gregor, I. M.; Haleem, M.; Hamnett, P. G.; Hiller, K. H.; Howarth, J.; Huang, Y.; Katzy, J.; Keller, J. S.; Kondrashova, N.; Kuhl, T.; Lobodzinska, E.; Lohwasser, K.; Madsen, A.; Medinnis, M.; Monig, K.; Garcia, R. F. Naranjo; Naumann, T.; O'Rourke, A. A.; Peschke, R.; Peters, K.; Pirumov, H.; Poley, A.; Robinson, J. E. M.; Schaefer, R.; Schmitt, S.; South, D.; Stanescu-Bellu, M.; Stanitzki, M. M.; Styles, N. A.; Tackmann, K.; Trofymov, A.; Wang, J.; Zakharchuk, N.] DESY, Zeuthen, Germany.
[Burmeister, I.; Cinca, D.; Dette, K.; Erdmann, J.; Esch, H.; Gossling, C.; Homann, M.; Klingenberg, R.; Kroeninger, K.] Tech Univ Dortmund, Inst Expt Phys 4, Dortmund, Germany.
[Anger, P.; Duschinger, D.; Friedrich, F.; Grohs, J. P.; Gutschow, C.; Hauswald, L.; Kobel, M.; Mader, W. F.; Novgorodova, O.; Siegert, F.; Socher, F.; Straessner, A.; Vest, A.; Wahrmund, S.] Tech Univ Dresden, Inst Kern & Teilchenphys, Dresden, Germany.
[Arce, A. T. H.; Benjamin, D. P.; Bjergaard, D. M.; Bocci, A.; Cerio, B. C.; Goshaw, A. T.; Kajomovitz, E.; Kotwal, A.; Kruse, M. C.; Li, L.; Li, S.; Liu, M.; Oh, S. H.; Zhou, C.] Duke Univ, Dept Phys, Durham, NC USA.
[Bristow, T. M.; Clark, P. J.; Dias, F. A.; Edwards, N. C.; Gao, Y.; Walls, F. M. Garay; Glayshers, P. C. F.; Harrington, R. D.; Leonidopoulos, C.; Martin, V. J.; Mijovic, L.; Mills, C.; Pino, S. A. Olivares; Washbrook, A.; Wynnes, B. M.] Univ Edinburgh, SUPA Sch Phys & Astron, Edinburgh, Midlothian, Scotland.
[Antonelli, M.; Beretta, M.; Bilokon, H.; Chiarella, V.; Curatolo, M.; Esposito, B.; Gatti, C.; Laurelli, P.; Maccarrone, G.; Mancini, G.; Sansoni, A.; Testa, M.; Vilucchi, E.] Ist Nazl Fis Nucl, Lab Nazl Frascati, Frascati, Italy.
[Arnold, H.; Betancourt, C.; Boehler, M.; Bruneliere, R.; Buehrer, F.; Burgard, C. D.; Buscher, D.; Cardillo, F.; Coniavitis, E.; Consorti, V.; Dang, N. P.; Dao, V.; Di Simone, A.; Gonella, G.; Herten, G.; Hirose, M.; Jakobs, K.; Javurek, T.; Jenni, P.; Kiss, F.; Koneke, K.; Kopp, A. K.; Kuehn, S.; Landgraf, U.; Luedtke, C.; Nagel, M.; Pagacova, M.; Parzefall, U.; Ronzani, M.; Rosbach, K.; Ruhr, F.; Rurikova, Z.; Sammel, D.; Schillo, C.; Schnoor, U.; Schumacher, M.; Son, H.; Sundermann, J. E.; Ta, D.; Temming, K. K.; Tsiskaridze, V.; Weiser, C.; Werner, M.; Zhang, L.; Zimmermann, S.] Albert Ludwigs Univ, Fak Math & Phys, Freiburg, Germany.
[Ancu, L. S.; De Mendizabal, J. Bilbao; Calace, N.; Chatterjee, A.; Clark, A.; Coccaro, A.; Delitzsch, C. M.; della Volpe, D.; Ferrere, D.; Gadomski, S.; Golling, T.; Gonzalez-Sevilla, S.; Gramling, J.; Guescini, F.; Iacobucci, G.; Katre, A.; Khoo, T. J.; Lanfermann, M. C.; Lionti, A. E.; March, L.; Mermod, P.; Miucci, A.; Nackenhorst, O.; Paolozzi, L.; Ristic, B.; Schramm, S.; Sfyrla, A.; Wu, X.] Univ Geneva, Sect Phys, Geneva, Switzerland.
[Barberis, D.; Darbo, G.; Favareto, A.; Parodi, A. Ferretto; Gagliardi, G.; Gaudiello, A.; Gemme, C.; Guido, E.; Miglioranzi, S.; Morettini, P.; Osculati, B.; Parodi, F.; Passaggio, S.; Rossi, L. P.; Sannino, M.; Schiavi, C.] Ist Nazl Fis Nucl, Sez Genova, Genoa, Italy.
[Barberis, D.; Favareto, A.; Parodi, A. Ferretto; Gagliardi, G.; Gaudiello, A.; Guido, E.; Miglioranzi, S.; Osculati, B.; Parodi, F.; Sannino, M.; Schiavi, C.] Univ Genoa, Dipartimento Fis, Genoa, Italy.
[Jejelava, J.; Tskhadadze, E. G.] Iv Javakhishvili Tbilisi State Univ, E Andronikashvili Inst Phys, Tbilisi, Rep of Georgia.
[Djobava, T.; Durglishvili, A.; Khubua, J.; Mosidze, M.] Tbilisi State Univ, Inst High Energy Phys, Tbilisi, Rep of Georgia.
[Duren, M.; Heinz, C.; Kreutzfeldt, K.; Stenzel, H.] Justus Liebig Univ Giessen, Inst Phys 2, Giessen, Germany.
[Bates, R. L.; Boutle, S. K.; Madden, W. D. Breaden; Britton, D.; Buckley, A. G.; Bussey, P.; Buttar, C. M.; Buzatu, A.; Crawley, S. J.; D'Auria, S.; Doyle, A. T.; Ferrando, J.; Gul, U.; Knue, A.; Mullen, P.; O'Shea, V.; Owen, M.; Pollard, C. S.; Qin, G.; Quilty, D.; Ravenscroft, T.; Robson, A.; St Denis, R. D.; Stewart, G. A.; Thompson, A. S.] Univ Glasgow, SUPA Sch Phys & Astron, Glasgow, Lanark, Scotland.
[Agricola, J.; Bindi, M.; Blumenschein, U.; Brandt, G.; De Maria, A.; Drechsler, E.; Graber, L.; Grosse-Knetter, J.; Janus, M.; Kareem, M. J.; Kawamura, G.; Lai, S.; Lemmer, B.; Magradze, E.; Mantoani, M.; Mchedlidze, G.; Llacer, M. Moreno; Musheghyan, H.; Quadt, A.; Rieger, J.; Rosien, N. -A.; Rzehorz, G. F.; Shabalina, E.; Stolte, P.; Veatch, J.; Weingarten, J.; Zinonos, Z.] Georg August Univ, Inst Phys 2, Gottingen, Germany.
[Albrand, S.; Berlendis, S.; Bethani, A.; Camincher, C.; Collot, J.; Crepe-Renaudin, S.; Delsart, P. A.; Gabaldon, C.; Genest, M. H.; Gradin, P. O. J.; Hostachy, J-Y.; Ledroit-Guillon, F.; Lleres, A.; Lucotte, A.; Malek, F.; Petit, E.; Stark, J.; Trocme, B.; Wu, M.] Univ Grenoble Alpes, Lab Phys Subatom & Cosmol, CNRS, IN2P3, Grenoble, France.
[Chan, S. K.; Clark, B. L.; Franklin, M.; Giromini, P.; Huth, J.; Ippolito, V.; Lazovich, T.; Mateos, D. Lopez; Morii, M.; Rogan, C. S.; Skottowe, H. P.; Sun, S.; Tolley, E.; Tong, B.; Tuna, A. N.; Yen, A. L.; Zambito, S.] Harvard Univ, Lab Particle Phys & Cosmol, Cambridge, MA 02138 USA.
[Andrei, V.; Antel, C.; Baas, A. E.; Brandt, O.; Djuvsland, J. I.; Dunford, M.; Geisler, M. P.; Hanke, P.; Jongmanns, J.; Kluge, E. -E.; Lang, V. S.; Meier, K.; Theenhausen, H. Meyer Zu; Villar, D. I. Narrias; Sahinsoy, M.; Scharf, V.; Schultz-Coulon, H. -C.; Stamen, R.; Starovoitov, P.; Suchek, S.; Wessels, M.] Heidelberg Univ, Kirchhoff Inst Phys, Heidelberg, Germany.
[Anders, C. F.; de Lima, A. D. E. Ferreira; Giulini, M.; Kolb, M.; Lisovyi, M.; Radescu, V.; Schaetzel, S.; Schoening, A.; Sosa, D.] Heidelberg Univ, Inst Phys, Heidelberg, Germany.
[Kretz, M.; Kugel, A.] Heidelberg Univ, ZITI Inst Tech Informat, Mannheim, Germany.
[Nagasaka, Y.] Hiroshima Inst Technol, Fac Appl Informat Sci, Hiroshima, Japan.
[Bortolotto, V.; Chan, Y. L.; Castillo, L. R. Flores; Lu, H.; Salvucci, A.; Tsui, K. M.] Chinese Univ Hong Kong, Dept Phys, Shatin, Hong Kong, Peoples R China.
[Bortolotto, V.; Orlando, N.; Tu, Y.] Univ Hong Kong, Dept Phys, Hong Kong, Hong Kong, Peoples R China.
[Bortolotto, V.; Prokofiev, K.] Hong Kong Univ Sci & Technol, Dept Phys, Kowloon, Hong Kong, Peoples R China.
[Choi, K.; Dattagupta, A.; Evans, H.; Gagnon, P.; Kopeliansky, R.; Lammers, S.; Martinez, N. Lorenzo; Luehring, F.; Ogren, H.; Penwell, J.; Weinert, B.; Zieminska, D.] Indiana Univ, Dept Phys, Bloomington, IN 47405 USA.
[Guenther, J.; Jansky, R.; Kneringer, E.; Lukas, W.; Milic, A.; Usanova, A.] Leopold Franzens Univ, Inst Astro & Teilchenphys, Innsbruck, Austria.
[Abdallah, J.; Argyropoulos, S.; Benitez, J.; Mallik, U.] Univ Iowa, Iowa City, IA USA.
[Chen, C.; Cochran, J.; De Lorenzi, F.; Jiang, H.; Krumnack, N.; Pluth, D.; Prell, S.; Werner, M. D.; Yu, J.] Iowa State Univ, Dept Phys & Astron, Ames, IA USA.
[Ahmadov, F.; Aleksandrov, I. N.; Bednyakov, V. A.; Boyko, I. R.; Budagov, I. A.; Chelkov, G. A.; Cheplakov, A.; Chizhov, M. V.; Dedovich, D. V.; Demichev, M.; Gongadze, A.; Gostkin, M. I.; Huseynov, N.; Javadov, N.; Karpov, S. N.; Karpova, Z. M.; Khramov, E.; Kruchonak, U.; Kukhtin, V.; Ladygin, E.; Lyubushkin, V.; Minashvili, I. A.; Mineev, M.; Peshekhonov, V. D.; Plotnikova, E.; Potrap, I. N.; Pozdnyakov, V.; Rusakovich, N. A.; Sadykov, R.; Sapronov, A.; Shiyakova, M.; Solovyanov, O. V.; Turchikhin, S.; Vinogradov, V. B.; Yeletskikh, I.; Zhemchugov, A.; Zimine, N. I.] JINR Dubna, Dubna, Russia.
[Amako, K.; Aoki, M.; Arai, Y.; Hanagaki, K.; Ikegami, Y.; Ikeno, M.; Iwasaki, H.; Kanzaki, J.; Kondo, T.; Kono, T.; Makida, Y.; Nagai, R.; Nagano, K.; Nakamura, K.; Nozaki, M.; Odaka, S.; Okuyama, T.; Sasaki, O.; Suzuki, S.; Takubo, Y.; Tanaka, S.; Terada, S.; Tokushuku, K.; Tsuno, S.; Unno, Y.; Yamamoto, A.; Yasu, Y.] KEK, High Energy Accelerator Res Org, Tsukuba, Ibaraki, Japan.
[Chen, Y.; Hasegawa, M.; Kido, S.; Kurashige, H.; Maeda, J.; Ochi, A.; Shimizu, S.; Yamazaki, Y.; Yuan, L.] Kobe Univ, Grad Sch Sci, Kobe, Hyogo, Japan.
[Kunigo, T.; Monden, R.; Sumida, T.; Tashiro, T.] Kyoto Univ, Fac Sci, Kyoto, Japan.
[Takashima, R.] Kyoto Univ, Kyoto, Japan.
[Kawagoe, K.; Oda, S.; Otono, H.; Tojo, J.] Kyushu Univ, Dept Phys, Fukuoka, Japan.
[Verzini, M. J. Alconada; Alonso, F.; Arduh, F. A.; Dova, M. T.; Monticelli, F.; Wahlberg, H.] Univ Nacl La Plata, Inst Fis La Plata, La Plata, Buenos Aires, Argentina.
[Verzini, M. J. Alconada; Alonso, F.; Arduh, F. A.; Dova, M. T.; Monticelli, F.; Wahlberg, H.] Consejo Nacl Invest Cient & Tecn, La Plata, Buenos Aires, Argentina.
[Barton, A. E.; Beattie, M. D.; Bertram, I. A.; Borissov, G.; Bouhova-Thacker, E. V.; Cheatham, S.; Dearnaley, W. J.; Fox, H.; Grimm, K.; Henderson, R. C. W.; Hughes, G.; Jones, R. W. L.; Kartvelishvili, V.; Long, R. E.; Love, P. A.; Muenstermann, D.; Parker, A. J.; Skinner, M. B.; Smizanska, M.; Walder, J.; Wharton, A. M.] Univ Lancaster, Dept Phys, Lancaster, England.
[Aliev, M.; Bachas, K.; Chiodini, G.; Gorini, E.; Longo, L.; Primavera, M.; Reale, M.; Spagnolo, S.; Ventura, A.] Ist Nazl Fis Nucl, Sez Lecce, Lecce, Italy.
[Aliev, M.; Bachas, K.; Gorini, E.; Longo, L.; Reale, M.; Spagnolo, S.; Ventura, A.] Univ Salento, Dipartimento Matemat & Fis, Lecce, Italy.
[Affolder, A. A.; Anders, J. K.; Burdin, S.; D'Onofrio, M.; Dervan, P.; Gwilliam, C. B.; Hayward, H. S.; Jones, T. J.; King, B. T.; Klein, M.; Klein, U.; Kretzschmar, J.; Laycock, P.; Lehan, A.; Maxfield, S. J.; Mehta, A.; Readioff, N. P.; Vossebeld, J. H.] Univ Liverpool, Oliver Lodge Lab, Liverpool, Merseyside, England.
[Cindro, V.; Deliyergiyev, M.; Filipcic, A.; Gorisek, A.; Kanjir, L.; Kersevan, B. P.; Kramberger, G.; Macek, B.; Mandic, I.; Mikuz, M.; Muskinja, M.; Sfiligoj, T.; Sokhrannyi, G.] Jozef Stefan Inst, Dept Phys, Ljubljana, Slovenia.
[Cindro, V.; Deliyergiyev, M.; Filipcic, A.; Gorisek, A.; Kanjir, L.; Kersevan, B. P.; Kramberger, G.; Macek, B.; Mandic, I.; Mikuz, M.; Muskinja, M.; Sfiligoj, T.; Sokhrannyi, G.] Univ Ljubljana, Ljubljana, Slovenia.
[Armitage, L. J.; Bevan, A. J.; Bona, M.; Hays, J. M.; Hickling, R.; Landon, M. P. J.; Lewis, D.; Lloyd, S. L.; Morris, J. D.; Nooney, T.; Piccaro, E.; Rizvi, E.; Sandbach, R. L.] Queen Mary Univ London, Sch Phys & Astron, London, England.
[Berry, T.; Boisvert, V.; Brooks, T.; Connelly, I. A.; Cowan, G.; Giannelli, M. Faucci; George, S.; Gibson, S. M.; Kempster, J. J.; Kilby, C. R.; Vazquez, J. G. Panduro; Pastore, Fr.; Savage, G.; Sowden, B. C.; Spano, F.; Teixeira-Dias, P.; Thomas-Wilsker, J.] Royal Holloway Univ London, Dept Phys, Surrey, England.
[Bell, A. S.; Butterworth, J. M.; Campanelli, M.; Christodoulou, V.; Cooper, B. D.; Davison, P.; Falla, R. J.; Freeborn, D.; Gregersen, K.; Ortiz, N. G. Gutierrez; Hesketh, G. G.; Jansen, E.; Jiggins, S.; Konstantinidis, N.; Korn, A.; Kucuk, H.; Leney, K. J. C.; Martyniuk, A. C.; McClymont, L. I.; Mcfayden, J. A.; Nurse, E.; Richter, S.; Scanlon, T.; Sekula, S. J.; Sherwood, P.; Simmons, B.; Wardrope, D. R.; Waugh, B. M.] UCL, Dept Phys & Astron, London, England.
[Greenwood, Z. D.; Grossi, G. C.; Jana, D. K.; Sawyer, L.] Louisiana Tech Univ, Ruston, LA 71270 USA.
[Beau, T.; Bomben, M.; Calderini, G.; Crescioli, F.; De Cecco, S.; Demilly, A.; Derue, F.; Francavilla, P.; Kaluza, A.; Krasny, M. W.; Lacour, D.; Laforge, B.; Laplace, S.; Le Dortz, O.; Lefebvre, G.; Solis, A. Lopez; Luzi, P. M.; Malaescu, B.; Marchiori, G.; Nikolic-Audit, I.; Ocariz, J.; Pandini, C. E.; Pires, S.; Ridel, M.; Roos, L.; Trincaz-Duvoid, S.; Varouchas, D.; Yap, Y. C.] UPMC, Lab Phys Nucl & Hautes Energies, Paris, France.
[Beau, T.; Bomben, M.; Calderini, G.; Crescioli, F.; De Cecco, S.; Demilly, A.; Derue, F.; Francavilla, P.; Kaluza, A.; Krasny, M. W.; Lacour, D.; Laforge, B.; Laplace, S.; Le Dortz, O.; Lefebvre, G.; Solis, A. Lopez; Luzi, P. M.; Malaescu, B.; Marchiori, G.; Nikolic-Audit, I.; Ocariz, J.; Pandini, C. E.; Pires, S.; Ridel, M.; Roos, L.; Trincaz-Duvoid, S.; Varouchas, D.; Yap, Y. C.] Univ Paris Diderot, Paris, France.
[Beau, T.; Bomben, M.; Calderini, G.; Crescioli, F.; De Cecco, S.; Demilly, A.; Derue, F.; Di Ciaccio, A.; Francavilla, P.; Kaluza, A.; Krasny, M. W.; Lacour, D.; Laforge, B.; Laplace, S.; Le Dortz, O.; Lefebvre, G.; Solis, A. Lopez; Luzi, P. M.; Malaescu, B.; Marchiori, G.; Nikolic-Audit, I.; Ocariz, J.; Pandini, C. E.; Pires, S.; Ridel, M.; Roos, L.; Sekula, S. J.; Trincaz-Duvoid, S.; Varouchas, D.; Yap, Y. C.] CNRS, IN2P3, Paris, France.
[Akesson, T. P. A.; Bocchetta, S. S.; Bryngemark, L.; Doglioni, C.; Floderus, A.; Hedberg, V.; Jarlskog, G.; Lytken, E.; Mjornmark, J. U.; Smirnova, O.; Viazlo, O.] Lund Univ, Fys Inst, Lund, Sweden.
[Barreiro, F.; Lopez, S. Calvente; Cueto, A.; De la Torre, H.; Del Peso, J.; Glasman, C.; Terron, J.] Univ Autonoma Madrid, Dept Fis Teor C15, Madrid, Spain.
[Artz, S.; Becker, M.; Bertella, C.; Blum, W.; Buscher, V.; Caputo, R.; Cuth, J.; Dimitrievska, A.; Dudder, A. Chr.; Endner, O. C.; Ertel, E.; Fiedler, F.; Torregrosa, E. Fullana; Geisen, M.; Groh, S.; Heck, T.; Jakobi, K. B.; Karnevskiy, M.; Kleinknecht, K.; Kopke, L.; Lin, T. H.; Masetti, L.; Mattmann, J.; Meyer, C.; Moritz, S.; Pleskot, V.; Rave, S.; Sander, H. G.; Schaeffer, J.; Schafer, U.; Schmitt, C.; Schmitz, S.; Schott, M.; Schuh, N.; Schulte, A.; Simioni, E.; Simon, M.; Tapprogge, S.; Urrejola, P.; Webb, S.; Yildirim, E.; Zimmermann, C.; Zinser, M.] Johannes Gutenberg Univ Mainz, Inst Phys, Mainz, Germany.
[Barnes, S. L.; Bielski, R.; Cox, B. E.; Da Via, C.; Dann, N. S.; Forcolin, G. T.; Forti, A.; Ponce, J. M. Iturbe; Li, X.; Loebinger, F. K.; Marsden, S. P.; Masik, J.; Sanchez, F. J. Munoz; Neep, T. J.; Oh, A.; Ospanov, R.; Pater, J. R.; Peters, R. F. Y.; Pilkington, A. D.; Pin, A. W. J.; Price, D.; Qin, Y.; Queitsch-Maitland, M.; Raine, J. A.; Schweiger, H.; Shaw, S. M.; Tomlinson, L.; Watts, S.; Wilk, F.; Woudstra, M. J.; Wyatt, T. R.] Univ Manchester, Sch Phys & Astron, Manchester, Lancs, England.
[Aad, G.; Alstaty, M.; Barbero, M.; Calandri, A.; Calvet, T. P.; Coadou, Y.; Diaconu, C.; Diglio, S.; Djama, F.; Ellajosyula, V.; Feligioni, L.; Gao, J.; Hadef, A.; Hallewell, G. D.; Hubaut, F.; Kahn, S. J.; Knoops, E. B. F. G.; Le Guirriec, E.; Liu, J.; Liu, K.; Madaffari, D.; Monnier, E.; Muanza, S.; Nagy, E.; Pralavorio, P.; Rodina, Y.; Rozanov, A.; Talby, M.; Theveneaux-Pelzer, T.; Torres, R. E. Ticse; Tisserant, S.; Toth, J.; Touchard, F.; Vacavant, L.; Wang, C.] Aix Marseille Univ, CPPM, Marseille, France.
[Aad, G.; Alstaty, M.; Barbero, M.; Calandri, A.; Calvet, T. P.; Coadou, Y.; Diaconu, C.; Diglio, S.; Djama, F.; Ellajosyula, V.; Feligioni, L.; Gao, J.; Hadef, A.; Hallewell, G. D.; Hubaut, F.; Kahn, S. J.; Knoops, E. B. F. G.; Le Guirriec, E.; Liu, J.; Liu, K.; Madaffari, D.; Monnier, E.; Muanza, S.; Nagy, E.; Pralavorio, P.; Rodina, Y.; Rozanov, A.; Talby, M.; Theveneaux-Pelzer, T.; Torres, R. E. Ticse; Tisserant, S.; Toth, J.; Touchard, F.; Vacavant, L.; Wang, C.] CNRS, IN2P3, Marseille, France.
[Bellomo, M.; Bernard, N. R.; Brau, B.; Dallapiccola, C.; Daya-Ishmukhametova, R. K.; Moyse, E. J. W.; Pais, P.; Pettersson, N. E.; Picazio, A.; Willocq, S.] Univ Massachusetts, Dept Phys, Amherst, MA USA.
[Belanger-Champagne, C.; Chuinard, A. J.; Corriveau, F.; Keyes, R. A.; Lefebvre, B.; Mantifel, R.; Prince, S.; Robertson, S. H.; Robichaud-Veronneau, A.; Stockton, M. C.; Stoebe, M.; Vachon, B.; Schroeder, T. Vazquez; Wang, K.; Warburton, A.] McGill Univ, Dept Phys, Montreal, PQ, Canada.
[Barberio, E. L.; Brennan, A. J.; Dawe, E.; Goldfarb, S.; Jennens, D.; Kubota, T.; Le, B.; McDonald, E. F.; Milesi, M.; Nuti, F.; Rados, P.; Scutti, F.; Spiller, L. A.; Tan, K. G.; Taylor, G. N.; Taylor, P. T. E.; Ungaro, F. C.; Urquijo, P.; Volpi, M.; Zanzi, D.] Univ Melbourne, Sch Phys, Melbourne, Vic, Australia.
[Amidei, D.; Chelstowska, M. A.; Cheng, H. C.; Dai, T.; Diehl, E. B.; Dimitrievska, A.; Edgar, R. C.; Feng, H.; Ferretti, C.; Fleischmann, P.; Guan, L.; Levin, D.; Liu, H.; Lu, N.; Marley, D. E.; Mc Kee, S. P.; McCarn, A.; Neal, H. A.; Qian, J.; Schwarz, T. A.; Searcy, J.; Sekhon, K.; Wu, Y.; Yu, J. M.; Zhang, D.; Zhou, B.; Zhu, J.] Univ Michigan, Dept Phys, Ann Arbor, MI 48109 USA.
[Arabidze, G.; Brock, R.; Chegwidden, A.; Fisher, W. C.; Halladjian, G.; Hauser, R.; Hayden, D.; Huston, J.; Martin, B.; Mondragon, M. C.; Plucinski, P.; Pope, B. G.; Schoenrock, B. D.; Schwienhorst, R.; Willis, C.] Michigan State Univ, Dept Phys & Astron, E Lansing, MI 48824 USA.
[Alimonti, G.; Andreazza, A.; Camplani, A.; Carminati, L.; Cavalli, D.; Citterio, M.; Costa, G.; Fanti, M.; Giugni, D.; Lari, T.; Lazzaroni, M.; Mandelli, L.; Manzoni, S.; Mazza, S. M.; Meroni, C.; Monzani, S.; Perini, L.; Ragusa, F.; Ratti, M. G.; Resconi, S.; Shojaii, S.; Stabile, A.; Tartarelli, G. F.; Troncon, C.; Turra, R.; Perez, M. Villaplana] Ist Nazl Fis Nucl, Sez Milano, Milan, Italy.
[Andreazza, A.; Camplani, A.; Carminati, L.; Fanti, M.; Lazzaroni, M.; Manzoni, S.; Mazza, S. M.; Monzani, S.; Perini, L.; Ragusa, F.; Ratti, M. G.; Shojaii, S.; Turra, R.; Perez, M. Villaplana] Univ Milan, Dipartimento Fis, Milan, Italy.
[Harkusha, S.; Kulchitsky, Y.; Kurochkin, Y. A.; Tsiareshka, P. V.] Natl Acad Sci Belarus, BI Stepanov Inst Phys, Minsk, Byelarus.
[Hrynevich, A.] Natl Sci & Educ Ctr Particle & High Energy Phys, Minsk, Byelarus.
[Arguin, J-F.; Azuelos, G.; Billoud, T. R. V.; Dallaire, F.; Ducu, O. A.; Gagnon, L. G.; Gauthier, L.; Leroy, C.; Mochizuki, K.; Manh, T. Nguyen; Rezvani, R.; Saadi, D. Shoaleh] Univ Montreal, Grp Particle Phys, Montreal, PQ, Canada.
[Akimov, A. V.; Gavrilenko, I. L.; Komar, A. A.; Mashinistov, R.; Mouraviev, S. V.; Nechaeva, P. Yu.; Shmeleva, A.; Snesarev, A. A.; Sulin, V. V.; Tikhomirov, V. O.; Zhukov, K.] Russian Acad Sci, PN Lebedev Phys Inst, Moscow, Russia.
[Artamonov, A.; Gorbounov, P. A.; Khovanskiy, V.; Shatalov, P. B.; Tsukerman, I. I.] ITEP, Moscow, Russia.
[Antonov, A.; Belotskiy, K.; Belyaev, N. L.; Bulekov, O.; Kantserov, V. A.; Krasnopevtsev, D.; Romaniouk, A.; Shulga, E.; Smirnov, S. Yu.; Smirnov, Y.; Soldatov, E. Yu.; Timoshenko, S.; Vorobev, K.] Natl Res Nucl Univ MEPhI, Moscow, Russia.
[Gladilin, L. K.; Kramarenko, V. A.; Maevskiy, A.; Sivoklokov, S. Yu.; Smirnova, L. N.] Moscow MV Lomonosov State Univ, DV Skobeltsyn Inst Nucl Phys, Moscow, Russia.
[Adomeit, S.; Bender, M.; Biebel, O.; Bock, C.; Calfayan, P.; Chow, B. K. B.; Duckeck, G.; Hartmannm, N. M.; Heinrich, J. J.; Hertenberger, R.; Hoenig, F.; Legger, F.; Lorenz, J.; Losel, P. J.; Maier, T.; Mann, A.; Mehlhase, S.; Meineck, C.; Mitrevski, J.; Mueller, R. S. P.; Rauscher, F.; Ruschke, A.; Schachtner, B. M.; Schaile, D.; Unverdorben, C.; Valderanis, C.; Walker, R.; Wittkowski, J.] Ludwig Maximilians Univ Munchen, Fak Phys, Munich, Germany.
[Barillari, T.; Bethke, S.; Compostella, G.; Cortiana, G.; Ecker, K. M.; Flowerdew, M. J.; Giuliani, C.; Ince, T.; Kiryunin, A. E.; Kluth, S.; Koehler, N. M.; Kortner, O.; Kortner, S.; Kroha, H.; La Rosa, A.; Macchiolo, A.; Maier, A. A.; McCarthy, T. G.; Menke, S.; Mueller, F.; Nisius, R.; Nowak, S.; Oberlack, H.; Richter, R.; Salihagic, D.; Sandstroem, R.; Savic, N.; Schacht, P.; Schmidt-Sommerfeld, K. R.; Spettel, F.; Stonjek, S.; Terzo, S.; von der Schmitt, H.; Wildauer, A.] Max Planck Inst Phys & Astrophys, Werner Heisenberg Inst, Munich, Germany.
[Fusayasu, T.; Shimojima, M.] Nagasaki Inst Appl Sci, Nagasaki, Japan.
[Horii, Y.; Kentaro, K.; Nakahama, Y.; Onogi, K.; Tomoto, M.; Wakabayashi, J.; Yamauchi, K.] Nagoya Univ, Grad Sch Sci, Nagoya, Aichi, Japan.
[Horii, Y.; Kentaro, K.; Nakahama, Y.; Onogi, K.; Tomoto, M.; Wakabayashi, J.; Yamauchi, K.] Nagoya Univ, Kobayashi Maskawa Inst, Nagoya, Aichi, Japan.
[Aloisio, A.; Alviggi, M. G.; Canale, V.; Carlino, G.; Cirotto, F.; Conventi, F.; de Asmundis, R.; Della Pietra, M.; Doria, A.; Izzo, V.; Merola, L.; Perrella, S.; Rossi, E.; Sanchez, A.; Sekhniaidze, G.] Ist Nazl Fis Nucl, Sez Napoli, Naples, Italy.
[Aloisio, A.; Alviggi, M. G.; Canale, V.; Cirotto, F.; Merola, L.; Perrella, S.; Rossi, E.; Sanchez, A.] Univ Napoli, Dipartimento Fis, Naples, Italy.
[Gorelov, I.; Hoeferkamp, M. R.; Mc Fadden, N. C.; Seidel, S. C.; Taylor, A. C.; Toms, K.] Univ New Mexico, Dept Phys & Astron, Albuquerque, NM 87131 USA.
[Caron, S.; Colasurdo, L.; Croft, V.; De Groot, N.; Filthaut, F.; Galea, C.; Konig, A. C.; Nektarijevic, S.; Strubig, A.] Radboud Univ Nijmegen, Nikhef, Inst Math Astrophys & Particle Phys, Nijmegen, Netherlands.
[Aben, R.; Angelozzi, I.; Bedognetti, M.; Beemster, L. J.; Bentvelsen, S.; Berge, D.; Bobbink, G. J.; Bos, K.; Brenner, L.; Bruni, L. S.; Butti, P.; Castelijn, R.; Castelli, A.; Colijn, A. P.; de Jong, P.; Deigaard, I.; Duda, D.; Ferrari, P.; Hartjes, F.; Hessey, N. P.; Igonkina, O.; Kluit, P.; Koffeman, E.; Mahlstedt, J.; Meyer, J.; Oussoren, K. P.; Sabato, G.; Salek, D.; Slawinska, M.; Valencic, N.; Van den Wollenberg, W.; Van der Deijl, P. C.; van der Graaf, H.; van Vulpen, I.; Vankov, P.; Verkerke, W.; Vermeulen, J. C.; Vreeswijk, M.; Weits, H.; Williams, S.; Wolfi, T. M. H.] Nikhef Natl Inst Subat Phys, Amsterdam, Netherlands.
[Aben, R.; Angelozzi, I.; Bedognetti, M.; Beemster, L. J.; Bentvelsen, S.; Berge, D.; Bobbink, G. J.; Bos, K.; Brenner, L.; Bruni, L. S.; Butti, P.; Castelijn, R.; Castelli, A.; Colijn, A. P.; de Jong, P.; Deigaard, I.; Duda, D.; Ferrari, P.; Hartjes, F.; Hessey, N. P.; Igonkina, O.; Kluit, P.; Koffeman, E.; Mahlstedt, J.; Meyer, J.; Oussoren, K. P.; Sabato, G.; Salek, D.; Slawinska, M.; Valencic, N.; Van den Wollenberg, W.; Van der Deijl, P. C.; van der Graaf, H.; van Vulpen, I.; Vankov, P.; Verkerke, W.; Vermeulen, J. C.; Vreeswijk, M.; Weits, H.; Williams, S.; Wolfi, T. M. H.] Univ Amsterdam, Amsterdam, Netherlands.
[Adelman, J.; Brost, E.; Burghgrave, B.; Chakraborty, D.; Klimek, P.; Saha, P.] Northern Illinois Univ, Dept Phys, De Kalb, IL USA.
[Anisenkov, A. V.; Baldin, E. M.; Bobrovnikov, V. S.; Bogdanchikov, A. G.; Buzykaev, A. R.; Kazanin, V. F.; Kharlamov, A. G.; Korol, A. A.; Maslennikov, A. L.; Maximov, D. A.; Peleganchuk, S. V.; Rezanova, O. L.; Soukharev, A. M.; Talyshev, A. A.; Tikhonov, Yu. A.] RAS, Budker Inst Nucl Phys, SB, Novosibirsk, Russia.
[Becot, C.; Bernius, C.; Cranmer, K.; Haas, A.; Heinrich, L.; Kaplan, B.; Karthik, K.; Konoplich, R.; Mincer, A. I.; Nemethy, P.; Neves, R. M.] NYU, Dept Phys, 4 Washington Pl, New York, NY 10003 USA.
[Beacham, J. B.; Che, S.; Gan, K. K.; Ishmukhametov, R.; Kagan, H.; Kass, R. D.; Looper, K. A.; Shrestha, S.; Tannenwald, B. B.] Ohio State Univ, Columbus, OH 43210 USA.
[Nakano, I.] Okayama Univ, Fac Sci, Okayama, Japan.
[Abbott, B.; Alhroob, M.; Bertsche, D.; De Benedetti, A.; Gutierrez, P.; Hasib, A.; Norberg, S.; Pearson, B.; Rifki, O.; Severini, H.; Skubic, P.; Strauss, M.] Univ Oklahoma, Homer L Dodge Dept Phys & Astron, Norman, OK 73019 USA.
[Cantero, J.; Haley, J.; Jamin, D. O.; Khanov, A.; Rizatdinova, F.; Sidorov, D.] Oklahoma State Univ, Dept Phys, Stillwater, OK 74078 USA.
[Chytka, L.; Hamal, P.; Hrabovsky, M.; Kvita, J.; Nozka, L.] Palacky Univ, RCPTM, Olomouc, Czech Republic.
[Abreu, R.; Allen, B. W.; Brau, J. E.; Hopkins, W. H.; Majewski, S.; Potter, C. T.; Radloff, P.; Sinev, N. B.; Strom, D. M.; Torrence, E.; Wanotayaroj, C.; Whalen, K.; Winklmeier, F.] Univ Oregon, Ctr High Energy Phys, Eugene, OR 97403 USA.
[Abeloos, B.; Ayoub, M. K.; Bassalat, A.; Binet, S.; Bourdarios, C.; De Regie, J. B. De Vivie; Delgove, D.; Duflot, L.; Escalier, M.; Fayard, L.; Fournier, D.; Gkougkousis, E. L.; Goudet, C. R.; Grivaz, J. -F.; Hariri, F.; Henrot-Versille, S.; Hrivnac, J.; Iconomidou-Fayard, L.; Kado, M.; Lounis, A.; Maiani, C.; Makovec, N.; Morange, N.; Nellist, C.; Petroff, P.; Poggioli, L.; Puzo, P.; Rousseau, D.; Rybkin, G.; Schaffer, A. C.; Serin, L.; Simion, S.; Tanaka, R.; Zerwas, D.; Zhang, Z.] Univ Paris Saclay, Univ Paris Sud, LAL, CNRS,IN2P3, Orsay, France.
[Ishijima, N.; Nomachi, M.; Sugaya, Y.; Teoh, J. J.; Yamaguchi, Y.] Osaka Univ, Grad Sch Sci, Osaka, Japan.
[Bugge, M. K.; Cameron, D.; Catmore, J. R.; Feigl, S.; Franconi, L.; Garonne, V.; Gjelsten, B. K.; Gramstad, E.; Morisbak, V.; Nilsen, J. K.; Ould-Saada, F.; Pajchel, K.; Pedersen, M.; Raddum, S.; Read, A. L.; Rohne, O.; Sandaker, H.; Serfon, C.; Stapnes, S.; Strandlie, A.] Univ Oslo, Dept Phys, Oslo, Norway.
[Artoni, G.; Barr, A. J.; Becker, K.; Beresford, L.; Bortoletto, D.; Burr, J. T. P.; Cooper-Sarkar, A. M.; Ortuzar, M. Crispin; Fawcett, W. J.; Frost, J. A.; Gallas, E. J.; Giuli, F.; Gupta, S.; Gwenlan, C.; Hays, C. P.; Henderson, J.; Huffman, T. B.; Issever, C.; Kalderon, C. W.; Nagai, K.; Nickerson, R. B.; Norjoharuddeen, N.; Petrov, M.; Pickering, M. A.; Tseng, J. C-L.; Viehhauser, G. H. A.; Vigani, L.; Weidberg, A. R.; Zhong, J.] Univ Oxford, Dept Phys, Oxford, England.
[Dondero, P.; Farina, E. M.; Ferrari, R.; Fraternali, M.; Gaudio, G.; Introzzi, G.; Lanza, A.; Livan, M.; Negri, A.; Polesello, G.; Rebuzzi, D. M.; Rimoldi, A.; Vercesi, V.] INFN, Sez Pavia, Pavia, Italy.
[Dondero, P.; Farina, E. M.; Fraternali, M.; Introzzi, G.; Livan, M.; Negri, A.; Rebuzzi, D. M.; Rimoldi, A.] Univ Pavia, Dipartimento Fis, Pavia, Italy.
[Balunas, W. K.; Brendlinger, K.; Di Clemente, W. K.; Fletcher, R. R. M.; Haney, B.; Heim, S.; Hines, E.; Jackson, B.; Kroll, J.; Lipeles, E.; Miguens, J. Machado; Meyer, C.; Mistry, K. P.; Reichert, J.; Thomson, E.; Vanguri, R.; Williams, H. H.; Yoshihara, K.] Univ Penn, Dept Phys, Philadelphia, PA 19104 USA.
[Basalaev, A.; Ezhilov, A.; Fedin, O. L.; Gratchev, V.; Levchenko, M.; Maleev, V. P.; Naryshkin, I.; Ryabov, Y. F.; Schegelsky, V. A.; Seliverstov, D. M.; Sommer, P.] BP Konstantinov Petersburg Nucl Phys Inst, Kurchatov Inst, Natl Res Ctr, St Petersburg, Russia.
[Annovi, A.; Bertolucci, F.; Biesuz, N. V.; Cavasinni, V.; Chiarelli, G.; Del Prete, T.; Dell'Orso, M.; Donati, S.; Giannetti, P.; Leone, S.; Roda, C.; Scuri, F.; Sotiropoulou, C. L.; Spalla, M.; Volpi, G.] INFN, Sez Pisa, Pisa, Italy.
[Annovi, A.; Bertolucci, F.; Biesuz, N. V.; Cavasinni, V.; Chiarelli, G.; Del Prete, T.; Dell'Orso, M.; Donati, S.; Giannetti, P.; Leone, S.; Roda, C.; Scuri, F.; Sotiropoulou, C. L.; Spalla, M.; Volpi, G.] Univ Pisa, Dipartimento Fis E Fermi, Pisa, Italy.
[Bianchi, R. M.; Boudreau, J.; Escobar, C.; Farina, C.; Hong, T. M.; Mueller, J.; Sapp, K.; Su, J.] Univ Pittsburgh, Dept Phys & Astron, Pittsburgh, PA 15260 USA.
[Aguilar-Saavedra, J. A.; Amor Dos Santos, S. P.; Amorim, A.; Araque, J. P.; Cantrill, R.; Carvalho, J.; Castro, N. F.; Muino, P. Conde; De Sousa, M. J. Da Cunha Sargedas; Fiolhais, M. C. N.; Galhardo, B.; Gomes, A.; Goncalo, R.; Jorge, P. M.; Lopes, L.; Maio, A.; Maneira, J.; Seabra, L. F. Oleiro; Onofre, A.; Pedro, R.; Santos, H.; Saraiva, J. G.; Silva, J.; Delgado, A. Tavares; Veloso, F.; Wolters, H.] Lab Instrumentacao & Fis Expt Particulas LIP, Lisbon, Portugal.
[Amorim, A.; Muino, P. Conde; De Sousa, M. J. Da Cunha Sargedas; Gomes, A.; Jorge, P. M.; Miguens, J. Machado; Maio, A.; Maneira, J.; Pedro, R.; Delgado, A. Tavares] Univ Lisbon, Fac Ciencias, Lisbon, Portugal.
[Amor Dos Santos, S. P.; Carvalho, J.; Fiolhais, M. C. N.; Galhardo, B.; Veloso, F.; Wolters, H.] Univ Coimbra, Dept Phys, Coimbra, Portugal.
[Gomes, A.; Maio, A.; Saraiva, J. G.; Silva, J.] Univ Lisbon, Ctr Fis Nucl, Lisbon, Portugal.
[Onofre, A.] Univ Minho, Dept Fis, Braga, Portugal.
[Aguilar-Saavedra, J. A.] Univ Granada, Dept Fis Teor & Cosmos, Granada, Spain.
[Aguilar-Saavedra, J. A.] Univ Granada, CAFPE, Granada, Spain.
Univ Nova Lisboa, Dept Fis, Caparica, Portugal.
Univ Nova Lisboa, CEFITEC, Fac Ciencias & Tecnol, Caparica, Portugal.
[Chudoba, J.; Havranek, M.; Hejbal, J.; Jakoubek, T.; Kepka, O.; Kupco, A.; Kus, V.; Lokajicek, M.; Lysak, R.; Marcisovsky, M.; Mikestikova, M.; Nemecek, S.; Penc, O.; Sicho, P.; Staroba, P.; Svatos, M.; Tasevsky, M.; Vrba, V.] Acad Sci Czech Republic, Inst Phys, Prague, Czech Republic.
[Ali, B.; Augsten, K.; Caforio, D.; Gallus, P.; Hubacek, Z.; Myska, M.; Pospisil, S.; Seifert, F.; Simak, V.; Slavicek, T.; Smolek, K.; Solar, M.; Sopko, V.; Suk, M.; Turecek, D.; Vacek, V.; Vlasak, M.; Vokac, P.; Vykydal, Z.; Zeman, M.] Czech Tech Univ, Prague, Czech Republic.
[Berta, P.; Carli, I.; Davidek, T.; Dolejsi, J.; Dolezal, Z.; Faltova, J.; Kodys, P.; Kosek, T.; Leitner, R.; Reznicek, P.; Scheirich, D.; Slovak, R.; Spousta, M.; Sykora, T.; Tas, P.; Todorova-Nova, S.; Valkar, S.; Vorobel, V.] Charles Univ Prague, Fac Math & Phys, Prague, Czech Republic.
[Borisov, A.; Cheremushkina, E.; Denisov, S. P.; Fakhrutdinov, R. M.; Fenyuk, A. B.; Golubkov, D.; Kamenshchikov, A.; Karyukhin, A. N.; Kozhin, A. S.; Minaenko, A. A.; Myagkov, A. G.; Nikolaenko, V.; Ryzhov, A.; Soloshenko, A.; Solovyev, V.; Starchenko, E. A.; Vaniachine, A.; Zaitsev, A. M.; Zenin, O.] NRC KI, State Res Ctr Inst High Energy Phys, Protvino, Russia.
[Adye, T.; Baines, J. T.; Barnett, B. M.; Burke, S.; Dewhurst, A.; Dopke, J.; Emeliyanov, D.; Gallop, B. J.; Gee, C. N. P.; Haywood, S. J.; Kirk, J.; Martin-Haugh, S.; McMahon, S. J.; Middleton, R. P.; Murray, W. J.; Phillips, P. W.; Sankey, D. P. C.; Sawyer, C.; Tyndel, M.; Wickens, F. J.; Wielers, M.; Worm, S. D.] Rutherford Appleton Lab, Particle Phys Dept, Didcot, Oxon, England.
[Anulli, F.; Bagiacchi, P.; Bagnaia, P.; Bauce, M.; Bini, C.; Ciapetti, G.; Corradi, M.; De Pedis, D.; De Salvo, A.; Di Donato, C.; Falciano, S.; Gentile, S.; Giagu, S.; Gustavino, G.; Kuna, M.; Lacava, F.; Luci, C.; Luminari, L.; Messina, A.; Nisati, A.; Pasqualucci, E.; Petrolo, E.; Pontecorvo, L.; Rescigno, M.; Rosati, S.; Tehrani, F. Safai; Vanadia, M.; Vari, R.; Veneziano, S.; Verducci, M.; Zanello, L.] Ist Nazl Fis Nucl, Sez Roma, Rome, Italy.
[Bagiacchi, P.; Bagnaia, P.; Bauce, M.; Bini, C.; Ciapetti, G.; Corradi, M.; Di Donato, C.; Gentile, S.; Giagu, S.; Gustavino, G.; Kuna, M.; Lacava, F.; Luci, C.; Messina, A.; Vanadia, M.; Verducci, M.; Zanello, L.] Sapienza Univ Roma, Dipartimento Fis, Rome, Italy.
[Aielli, G.; Camarri, P.; Cardarelli, R.; Cerrito, L.; Di Ciaccio, A.; Luppa, R.; Liberti, B.; Salamon, A.; Santonico, R.] INFN, Sez Roma Tor Vergata, Rome, Italy.
[Aielli, G.; Camarri, P.; Cerrito, L.; Di Ciaccio, A.; Luppa, R.; Salamon, A.; Santonico, R.] Univ Roma Tor Vergata, Dipartimento Fis, Rome, Italy.
[Baroncelli, A.; Biglietti, M.; Ceradini, F.; Di Micco, B.; Farilla, A.; Graziani, E.; Iodice, M.; Orestano, D.; Petrucci, F.; Puddu, D.; Salamanna, G.; Sessa, M.; Stanescu, C.; Taccini, C.] INFN, Sez Roma Tre, Rome, Italy.
[Ceradini, F.; Di Micco, B.; Orestano, D.; Petrucci, F.; Puddu, D.; Salamanna, G.; Sessa, M.; Taccini, C.] Univ Roma Tre, Dipartimento Matemat & Fis, Rome, Italy.
[Benchekroun, D.; Chafaq, A.; Hoummada, A.] Univ Hassan 2, Res Univ Phys Hautes Energies, Fac Sci Ain Chock, Casablanca, Morocco.
[Ghazlane, H.] Ctr Natl Energie Sci Tech Nucl, Rabat, Morocco.
[El Kacimi, M.; Goujdami, D.] Univ Cadi Ayyad, LPHEA Marrakech, Fac Sci Semlalia, Marrakech, Morocco.
[Aaboud, M.; Derkaoui, J. E.; Ouchrif, M.] Univ Mohamed Premier, Fac Sci, Oujda, Morocco.
[Aaboud, M.; Derkaoui, J. E.; Ouchrif, M.] LPTPM, Oujda, Morocco.
[El Moursli, R. Cherkaoui; Fassi, F.; Haddad, N.; Idrissi, Z.; Tayalati, Y.] Univ Mohammed 5, Fac Sci, Rabat, Morocco.
[Bachacou, H.; Balli, F.; Bauer, F.; Besson, N.; Blanchard, J. -B.; Boonekamp, M.; Chevalier, L.; Hoffmann, M. Dano; Deliot, F.; Denysiuk, D.; Etienvre, A. I.; Formica, A.; Giraud, P. F.; Da Costa, J. Goncalves Pinto Firmino; Guyot, C.; Hanna, R.; Hassani, S.; Jeanneau, F.; Kivernyk, O.; Kozanecki, W.; Kukla, R.; Lancon, E.; Laporte, J. F.; Le Quilleuc, E. P.; Lesage, A. A. J.; Mansoulie, B.; Meyer, J-P; Nicolaidou, R.; Ouraou, A.; Rodriguez, L. Pacheco; Perego, M. M.; Peyaud, A.; Royon, C. R.; Saimpert, M.; Schoeffel, L.; Schune, Ph.; Schwemling, Ph.; Schwindling, J.] CEA Saclay, DSM IRFU Inst Rech Lois Fondamentales Univers, Gif Sur Yvette, France.
[AbouZeid, O. S.; Battaglia, M.; Debenedetti, C.; Grillo, A. A.; Hance, M.; Kuhl, A.; Law, A. T.; Litke, A. M.; Lockman, W. S.; Nielsen, J.; Reece, R.; Rose, P.; Sadrozinski, H. F-W.; Schier, S.; Schumm, B. A.; Seiden, A.] Univ Calif Santa Cruz, Santa Cruz Inst Particle Phys, Santa Cruz, CA 95064 USA.
[Alpigiani, C.; Blackburn, D.; Goussiou, A. G.; Hsu, S. -C.; Johnson, W. J.; Lubatti, H. J.; Marx, M.; Meehan, S.; Rompotis, N.; Rosten, R.; Rothberg, J.; Russell, H. L.; De Bruin, P. H. Sales; Pastor, E. Torro; Watts, G.; Whallon, N. L.] Univ Washington, Dept Phys, Seattle, WA 98195 USA.
[Anastopoulos, C.; Costanzo, D.; Donszelmann, T. Cuhadar; Dawson, I.; Fletcher, G. T.; Hamity, G. N.; Hodgkinson, M. C.; Hodgson, P.; Johansson, P.; Klinger, J. A.; Korolkova, E. V.; Kyriazopoulos, D.; Paredes, B. Lopez; Macdonald, C. M.; Miyagawa, P. S.; Parker, K. A.; Tovey, D. R.; Vickey, T.; Boeriu, O. E. Vickey] Univ Sheffield, Dept Phys & Astron, Sheffield, S Yorkshire, England.
[Hasegawa, Y.; Takeshita, T.] Shinshu Univ, Dept Phys, Nagano, Japan.
[Atlay, N. B.; Buchholz, P.; Campoverde, A.; Czirr, H.; Fleck, I.; Ghasemi, S.; Ibragimov, I.; Li, Y.; Rosenthal, O.; Walkowiak, W.; Ziolkowski, M.] Univ Siegen, Fachbereich Phys, Siegen, Germany.
[Buat, Q.; Horton, A. J.; Mori, D.; O'Neil, D. C.; Pachal, K.; Stelzer, B.; Temple, D.; Torres, H.; Van Nieuwkoop, J.; Vetterli, M. C.] Simon Fraser Univ, Dept Phys, Burnaby, BC, Canada.
[Armbruster, A. J.; Barklow, T.; Bartoldus, R.; Bawa, H. S.; Black, J. E.; Dimitrievska, A.; Gao, Y. S.; Garelli, N.; Grenier, P.; Ilic, N.; Kagan, M.; Kocian, M.; Koi, T.; Malone, C.; Moss, J.; Mount, R.; Nachman, B. P.; Piacquadio, G.; Rubbo, F.; Salnikov, A.; Schwartzman, A.; Su, D.; Tompkins, L.; Wittgen, M.; Young, C.; Zeng, Q.] SLAC Natl Accelerator Lab, Stanford, CA USA.
[Astalos, R.; Bartos, P.; Blazek, T.; Dado, T.; Melo, M.; Plazak, L.; Smiesko, J.; Sykora, I.; Tokar, S.; Zenis, T.] Comenius Univ, Fac Math Phys & Informat, Bratislava, Slovakia.
[Bruncko, D.; Kladiva, E.; Strizenec, P.; Urban, J.] Slovak Acad Sci, Inst Expt Phys, Dept Subnucl Phys, Kosice, Slovakia.
[Castaneda-Miranda, E.; Hamilton, A.; Yacoob, S.] Univ Cape Town, Dept Phys, Cape Town, South Africa.
[Connell, S. H.; Govender, N.] Univ Johannesburg, Dept Phys, Johannesburg, South Africa.
[Hsu, C.; Kar, D.; Garcia, B. R. Mellado; Ruan, X.] Univ Witwatersrand, Sch Phys, Johannesburg, South Africa.
[Akerstedt, H.; Asman, B.; Bendtz, K.; Bertoli, G.; Bylund, O. Bessidskaia; Bohm, C.; Clement, C.; Hellman, S.; Jon-And, K.; Lundberg, O.; Milstead, D. A.; Molander, S.; Pani, P.; Poettgen, R.; Shaikh, N. W.; Shcherbakova, A.; Sjolin, J.; Strandberg, S.; Ughetto, M.; Santurio, E. Valdes] Stockholm Univ, Dept Phys, Stockholm, Sweden.
[Abulaiti, Y.; Akerstedt, H.; Asman, B.; Bendtz, K.; Bertoli, G.; Bylund, O. Bessidskaia; Clement, C.; Cribbs, W. A.; Hellman, S.; Jon-And, K.; Lundberg, O.; Milstead, D. A.; Moa, T.; Molander, S.; Pani, P.; Poettgen, R.; Rossetti, V.; Shaikh, N. W.; Shcherbakova, A.; Sjolin, J.; Strandberg, S.; Ughetto, M.; Santurio, E. Valdes; Wallangen, V.] Oskar Klein Ctr, Stockholm, Sweden.
[Lund-Jensen, B.; Sidebo, P. E.; Strandberg, J.] Royal Inst Technol, Dept Phys, Stockholm, Sweden.
[Backes, M.; Balestri, T.; Bee, C. P.; Chen, K.; Hobbs, J.; Huo, P.; Jia, J.; Li, H.; Lindquist, B. E.; McCarthy, R. L.; Montalbano, A.; Morvaj, L.; Radhakrishnan, S. K.; Rijssenbeek, M.; Schamberger, R. D.; Tsybychev, D.; Zaman, A.; Zhou, M.] SUNY Stony Brook, Dept Phys & Astron, Stony Brook, NY 11794 USA.
[Backes, M.; Balestri, T.; Bee, C. P.; Chen, K.; Hobbs, J.; Huo, P.; Jia, J.; Li, H.; Lindquist, B. E.; McCarthy, R. L.; Montalbano, A.; Morvaj, L.; Radhakrishnan, S. K.; Rijssenbeek, M.; Schamberger, R. D.; Tsybychev, D.; Zaman, A.; Zhou, M.] SUNY Stony Brook, Dept Chem, Stony Brook, NY 11794 USA.
[Abraham, N. L.; Allbrooke, B. M. M.; Asquith, L.; Cerri, A.; Barajas, C. A. Chavez; De Sanctis, U.; De Santo, A.; Grout, Z. J.; Lerner, G.; Miano, F.; Salvatore, F.; Castillo, I. Santoyo; Shehu, C. Y.; Suruliz, K.; Sutton, M. R.; Vivarelli, I.; Winston, O. J.] Univ Sussex, Dept Phys & Astron, Brighton, E Sussex, England.
[Black, C. W.; Finelli, K. D.; Jeng, G. -Y.; Limosani, A.; Morley, A. K.; Saavedra, A. F.; Scarcella, M.; Varvell, K. E.; Wang, J.; Yabsley, B.] Univ Sydney, Sch Phys, Sydney, NSW, Australia.
[Hou, S.; Hsu, P. J.; Lee, S. C.; Lin, S. C.; Liu, B.; Liu, D.; Lo Sterzo, F.; Mazini, R.; Shi, L.; Soh, D. A.; Teng, P. K.; Wang, S. M.; Yang, Y.] Acad Sinica, Inst Phys, Taipei, Taiwan.
[Abreu, H.; Gozani, E.; Rozen, Y.; Tarem, S.; van Eldik, N.] Technion Israel Inst Technol, Dept Phys, Haifa, Israel.
[Abramowicz, H.; Alexander, G.; Ashkenazi, A.; Bella, G.; Benary, O.; Benhammou, Y.; Davies, M.; Duarte-Campderros, J.; Etzion, E.; Gershon, A.; Gueta, O.; Oren, Y.; Soffer, A.; Taiblum, N.] Tel Aviv Univ, Raymond & Beverly Sackler Sch Phys & Astron, Tel Aviv, Israel.
[Gentsos, C.; Gkaitatzis, S.; Gkialas, I.; Iliadis, D.; Kimura, N.; Kordas, K.; Kourkoumeli-Charalampidi, A.; Leisos, A.; Papageorgiou, K.; Petridou, C.; Sampsonidis, D.] Aristotle Univ Thessaloniki, Dept Phys, Thessaloniki, Greece.
[Asai, S.; Chen, S.; Enari, Y.; Hanawa, K.; Ishino, M.; Kanaya, N.; Kataoka, Y.; Kato, C.; Kawamoto, T.; Kishimoto, T.; Kobayashi, A.; Kobayashi, T.; Komori, Y.; Kozakai, C.; Mashimo, T.; Masubuchi, T.; Minami, Y.; Mori, T.; Morinaga, M.; Nakamura, T.; Ninomiya, Y.; Nobe, T.; Okumura, Y.; Saito, T.; Sakamoto, H.; Sasaki, Y.; Tanaka, J.; Terashi, K.; Ueda, I.; Yamamoto, S.; Yamanaka, T.] Univ Tokyo, Int Ctr Elementary Particle Phys, Tokyo, Japan.
[Asai, S.; Chen, S.; Enari, Y.; Hanawa, K.; Ishino, M.; Kanaya, N.; Kataoka, Y.; Kato, C.; Kawamoto, T.; Kishimoto, T.; Kobayashi, A.; Kobayashi, T.; Komori, Y.; Kozakai, C.; Mashimo, T.; Masubuchi, T.; Minami, Y.; Mori, T.; Morinaga, M.; Nakamura, T.; Ninomiya, Y.; Nobe, T.; Okumura, Y.; Saito, T.; Sakamoto, H.; Sasaki, Y.; Tanaka, J.; Terashi, K.; Ueda, I.; Yamamoto, S.; Yamanaka, T.] Univ Tokyo, Dept Phys, Tokyo, Japan.
[Bratzler, U.; Fukunaga, C.] Tokyo Metropolitan Univ, Grad Sch Sci & Technol, Tokyo, Japan.
[Hayakawa, D.; Ishitsuka, M.; Jinnouchi, O.; Kobayashi, D.; Kuze, M.; Motohashi, K.; Tanaka, M.; Todome, K.; Yamaguchi, D.] Tokyo Inst Technol, Dept Phys, Tokyo, Japan.
[Batista, S. J.; Chau, C. C.; Cormier, K. J. R.; DeMarco, D. A.; Di Sipio, R.; Diamond, M.; Keoshkerian, H.; Krieger, P.; Liblong, A.; Mc Goldrick, G.; Orr, R. S.; Pascuzzi, V. R.; Polifka, R.; Rudolph, M. S.; Savard, P.; Sinervo, P.; Taenzer, J.; Teuscher, R. J.; Trischuk, W.; Veloce, L. M.; Venturi, N.] Univ Toronto, Dept Phys, Toronto, ON, Canada.
[Canepa, A.; Chekulaev, S. V.; Hod, N.; Jovicevic, J.; Codina, E. Perez; Schneider, B.; Stelzer-Chilton, O.; Tafirout, R.; Trigger, I. M.] TRIUMF, Vancouver, BC, Canada.
[Ramos, J. Manjarres; Palacino, G.; Taylor, W.] York Univ, Dept Phys & Astron, Toronto, ON, Canada.
[Hara, K.; Ito, F.; Kasahara, K.; Kim, S. H.; Kiuchi, K.; Nagata, K.; Okawa, H.; Sato, K.; Ukegawa, F.] Univ Tsukuba, Fac Pure & Appl Sci, Tsukuba, Ibaraki, Japan.
[Hara, K.; Ito, F.; Kasahara, K.; Kim, S. H.; Kiuchi, K.; Nagata, K.; Okawa, H.; Sato, K.; Ukegawa, F.] Univ Tsukuba, Ctr Integrated Res Fundamental Sci & Engn, Tsukuba, Ibaraki, Japan.
[Beauchemin, P. H.; Meoni, E.; Sliwa, K.; Song, H. Y.; Wetter, J.] Tufts Univ, Dept Phys & Astron, Medford, MA 02155 USA.
[Casper, D. W.; Corso-Radu, A.; Frate, M.; Guest, D.; Lankford, A. J.; Mete, A. S.; Nelson, A.; Scannicchio, D. A.; Schernau, M.; Shimmin, C. O.; Taffard, A.; Unel, G.; Whiteson, D.] Univ Calif Irvine, Dept Phys & Astron, Irvine, CA USA.
[Acharya, B. S.; Boldyrev, A. S.; Cobal, M.; Giordani, M. P.; Pinamonti, M.; Quayle, W. B.; Serkin, L.; Shaw, K.; Soualah, R.; Truong, L.] INFN, Grp Collegato Udine, Sez Trieste, Udine, Italy.
[Acharya, B. S.; Quayle, W. B.; Serkin, L.; Shaw, K.] Abdus Salaam Int Ctr Theoret Phys, Trieste, Italy.
[Boldyrev, A. S.; Cobal, M.; Giordani, M. P.; Pinamonti, M.; Soualah, R.; Truong, L.] Univ Udine, Dipartimento Chim Fis & Ambiente, Udine, Italy.
[Kuutmann, E. Bergeaas; Brenner, R.; Ekelof, T.; Ellert, M.; Ferrari, A.; Maddocks, H. J.; Ohman, H.; Rangel-Smith, C.] Uppsala Univ, Dept Phys & Astron, Uppsala, Sweden.
[Atkinson, M.; Armadans, R. Caminal; Cavaliere, V.; Chang, P.; Errede, S.; Hooberman, B. H.; Khader, M.; Lie, K.; Liss, T. M.; Liu, L.; Long, J. D.; Outschoorn, V. I. Martinez; Neubauer, M. S.; Rybar, M.; Shang, R.; Sickles, A. M.; Vichou, I.; Zeng, J. C.] Univ Illinois, Dept Phys, 1110 W Green St, Urbana, IL 61801 USA.
[Alvarez Piqueras, D.; Barranco Navarro, L.; Urban, S. Cabrera; Gimenez, V. Castillo; Alberich, L. Cerda; Costa, M. J.; Martinez, P. Fernandez; Ferrer, A.; Fiorini, L.; Fuster, J.; Garcia, C.; Navarro, J. E. Garcia; Gonzalez de la Hoz, S.; Jimenez, Y. Hernandez; Higon-Rodriguez, E.; Pena, J. Jimenez; King, M.; Lacasta, C.; Lacuesta, V. R.; Mamuzic, J.; Marti-Garcia, S.; Melini, D.; Mitsou, V. A.; Lopez, S. Pedraza; Rodriguez, D. Rodriguez; Adam, E. Romero; Ros, E.; Salt, J.; Sanchez, J.; Martinez, V. Sanchez; Soldevila, U.; Valero, A.; Ferrer, J. A. Valls; Vos, M.] Univ Valencia, IFIC, Valencia, Spain.
[Alvarez Piqueras, D.; Barranco Navarro, L.; Urban, S. Cabrera; Gimenez, V. Castillo; Alberich, L. Cerda; Costa, M. J.; Martinez, P. Fernandez; Ferrer, A.; Fiorini, L.; Fuster, J.; Garcia, C.; Navarro, J. E. Garcia; Gonzalez de la Hoz, S.; Jimenez, Y. Hernandez; Higon-Rodriguez, E.; Pena, J. Jimenez; King, M.; Lacasta, C.; Lacuesta, V. R.; Mamuzic, J.; Marti-Garcia, S.; Melini, D.; Mitsou, V. A.; Lopez, S. Pedraza; Rodriguez, D. Rodriguez; Adam, E. Romero; Ros, E.; Salt, J.; Sanchez, J.; Martinez, V. Sanchez; Soldevila, U.; Valero, A.; Ferrer, J. A. Valls; Vos, M.] Univ Valencia, Dept Fis Atom Mol & Nucl, Valencia, Spain.
[Alvarez Piqueras, D.; Barranco Navarro, L.; Urban, S. Cabrera; Gimenez, V. Castillo; Alberich, L. Cerda; Costa, M. J.; Martinez, P. Fernandez; Ferrer, A.; Fiorini, L.; Fuster, J.; Garcia, C.; Navarro, J. E. Garcia; Gonzalez de la Hoz, S.; Jimenez, Y. Hernandez; Higon-Rodriguez, E.; Pena, J. Jimenez; King, M.; Lacasta, C.; Lacuesta, V. R.; Mamuzic, J.; Marti-Garcia, S.; Melini, D.; Mitsou, V. A.; Lopez, S. Pedraza; Rodriguez, D. Rodriguez; Adam, E. Romero; Ros, E.; Salt, J.; Sanchez, J.; Martinez, V. Sanchez; Soldevila, U.; Valero, A.; Ferrer, J. A. Valls; Vos, M.] Univ Valencia, Dept Ingn Elect, Valencia, Spain.
[Alvarez Piqueras, D.; Barranco Navarro, L.; Urban, S. Cabrera; Gimenez, V. Castillo; Alberich, L. Cerda; Costa, M. J.; Martinez, P. Fernandez; Ferrer, A.; Fiorini, L.; Fuster, J.; Garcia, C.; Navarro, J. E. Garcia; Gonzalez de la Hoz, S.; Jimenez, Y. Hernandez; Higon-Rodriguez, E.; Pena, J. Jimenez; King, M.; Lacasta, C.; Lacuesta, V. R.; Mamuzic, J.; Marti-Garcia, S.; Melini, D.; Mitsou, V. A.; Lopez, S. Pedraza; Rodriguez, D. Rodriguez; Adam, E. Romero; Ros, E.; Salt, J.; Sanchez, J.; Martinez, V. Sanchez; Soldevila, U.; Valero, A.; Ferrer, J. A. Valls; Vos, M.] Univ Valencia, Inst Microelect Barcelona IMB CNM, Valencia, Spain.
[Alvarez Piqueras, D.; Barranco Navarro, L.; Urban, S. Cabrera; Gimenez, V. Castillo; Alberich, L. Cerda; Costa, M. J.; Martinez, P. Fernandez; Ferrer, A.; Fiorini, L.; Fuster, J.; Garcia, C.; Navarro, J. E. Garcia; Gonzalez de la Hoz, S.; Jimenez, Y. Hernandez; Higon-Rodriguez, E.; Pena, J. Jimenez; King, M.; Lacasta, C.; Lacuesta, V. R.; Mamuzic, J.; Marti-Garcia, S.; Melini, D.; Mitsou, V. A.; Lopez, S. Pedraza; Rodriguez, D. Rodriguez; Adam, E. Romero; Ros, E.; Salt, J.; Sanchez, J.; Martinez, V. Sanchez; Soldevila, U.; Valero, A.; Ferrer, J. A. Valls; Vos, M.] CSIC, Valencia, Spain.
[Danninger, M.; Fedorko, W.; Gay, C.; Gecse, Z.; Gignac, M.; Henkelmann, S.; King, S. B.; Lister, A.] Univ British Columbia, Dept Phys, Vancouver, BC, Canada.
[Albert, J.; David, C.; Elliot, A. A.; Fincke-Keeler, M.; Hamano, K.; Hill, E.; Keeler, R.; Kowalewski, R.; Kuwertz, E. S.; Kwan, T.; LeBlanc, M.; Lefebvre, M.; McPherson, R. A.; Pearce, J.; Seuster, R.; Sobie, R.; Trovatelli, M.; Venturi, M.] Univ Victoria, Dept Phys & Astron, Victoria, BC, Canada.
[Beckingham, M.; Ennis, J. S.; Farrington, S. M.; Harrison, P. F.; Jeske, C.; Jones, G.; Martin, T. A.; Murray, W. J.; Pianori, E.; Spangenberg, M.] Univ Warwick, Dept Phys, Coventry, W Midlands, England.
[Iizawa, T.; Kaji, T.; Mitani, T.; Sakurai, Y.; Yorita, K.] Waseda Univ, Tokyo, Japan.
[Balek, P.; Bressler, S.; Citron, Z. H.; Duchovni, E.; Dumancic, M.; Gross, E.; Kohler, M. K.; Lellouch, D.; Levinson, L. J.; Mikenberg, G.; Milov, A.; Pitt, M.; Ravinovich, I.; Roth, I.; Schaarschmidt, J.; Smakhtin, V.; Turgeman, D.] Weizmann Inst Sci, Dept Particle Phys, Rehovot, Israel.
[Banerjee, Sw.; Guan, W.; Hard, A. S.; Heng, Y.; Ji, H.; Ju, X.; Kaplan, L. S.; Kashif, L.; Kruse, A.; Ming, Y.; Wang, F.; Wiedenmann, W.; Wu, S. L.; Yang, H.; Zhang, F.; Zobernig, G.] Univ Wisconsin, Dept Phys, 1150 Univ Ave, Madison, WI 53706 USA.
[Herget, V.; Kuger, F.; Redelbach, A.; Schreyer, M.; Sidiropoulou, O.; Siragusa, G.; Strohmer, R.; Trefzger, T.; Weber, S. W.; Zibell, A.] Julius Maximilians Univ, Fak Phys & Astron, Wurzburg, Germany.
[Bannoura, A. A. E.; Boerner, D.; Braun, H. M.; Cornelissen, T.; Ellinghaus, F.; Ernis, G.; Fischer, J.; Flick, T.; Gabizon, O.; Gilles, G.; Hamacher, K.; Harenberg, T.; Hirschbuehl, D.; Kersten, S.; Kuechler, J. T.; Mattig, P.; Neumann, M.; Pataraia, S.; Riegel, C. J.; Sandhoff, M.; Tepel, F.; Vogel, M.; Wagner, W.; Zeitnitz, C.] Berg Univ Wuppertal, Facegrp Phys, Fak Math & Nat Wissensch, Wuppertal, Germany.
[Baker, O. K.; Noccioli, E. Benhar; Cummings, J.; Demers, S.; Ideal, E.; Lagouri, T.; Leister, A. G.; Loginov, A.; Hernandez, D. Paredes; Thomsen, L. A.; Tipton, P.; Vasquez, J. G.; Wang, X.] Yale Univ, Dept Phys, New Haven, CT USA.
[Hakobyan, H.; Vardanyan, G.] Yerevan Phys Inst, Yerevan, Armenia.
[Rahal, G.] Ctr Calcul, IN2P3, Villeurbanne, France.
[Acharya, B. S.] Kings Coll London, Dept Phys, London, England.
[Ahmadov, F.; Huseynov, N.; Javadov, N.] Azerbaijan Acad Sci, Inst Phys, Baku, Azerbaijan.
[Anisenkov, A. V.; Baldin, E. M.; Bobrovnikov, V. S.; Buzykaev, A. R.; Kazanin, V. F.; Kharlamov, A. G.; Korol, A. A.; Maslennikov, A. L.; Maximov, D. A.; Peleganchuk, S. V.; Rezanova, O. L.; Soukharev, A. M.; Talyshev, A. A.; Tikhonov, Yu. A.] Novosibirsk State Univ, Novosibirsk, Russia.
[Azuelos, G.; Gingrich, D. M.; Oakham, F. G.; Savard, P.; Vetterli, M. C.] TRIUMF, Vancouver, BC, Canada.
[Banerjee, Sw.] Univ Louisville, Dept Phys & Astron, Louisville, KY 40292 USA.
[Bawa, H. S.; Gao, Y. S.] Calif State Univ Fresno, Dept Phys, Fresno, CA 93740 USA.
[Beck, H. P.] Univ Fribourg, Dept Phys, Fribourg, Switzerland.
[Casado, M. P.] Univ Autonoma Barcelona, Dept Fis, Barcelona, Spain.
[Castro, N. F.] Univ Porto, Fac Ciencias, Dept Fis & Astron, Oporto, Portugal.
[Chelkov, G. A.] Tomsk State Univ, Tomsk, Russia.
[Conventi, F.; Della Pietra, M.] Univ Napoli Parthenope, Naples, Italy.
[Corriveau, F.; McPherson, R. A.; Sobie, R.; Teuscher, R. J.] IPP, Toronto, ON, Canada.
[Ducu, O. A.] Natl Inst Phys & Nucl Engn, Bucharest, Romania.
[Fedin, O. L.] St Petersburg State Polytech Univ, Dept Phys, St Petersburg, Russia.
[Geng, C.; Guo, Y.; Li, B.] Univ Michigan, Dept Phys, Ann Arbor, MI 48109 USA.
[Govender, N.] Ctr High Performance Comp, CSIR Campus, Cape Town, South Africa.
[Greenwood, Z. D.; Sawyer, L.] Louisiana Tech Univ, Ruston, LA 71270 USA.
[Grinstein, S.; Rozas, A. Juste; Martinez, M.] ICREA, Barcelona, Spain.
[Hanagaki, K.] Osaka Univ, Grad Sch Sci, Osaka, Japan.
[Hsu, P. J.] Natl Tsing Hua Univ, Dept Phys, Hsinchu, Taiwan.
[Igonkina, O.] Radboud Univ Nijmegen, Nikhef, Inst Math Astrophys & Particle Phys, Nijmegen, Netherlands.
[Ilchenko, Y.; Onyisi, P. U. E.] Univ Texas Austin, Dept Phys, Austin, TX 78712 USA.
[Jejelava, J.] Ilia State Univ, Inst Theoret Phys, Tbilisi, Rep of Georgia.
[Jenni, P.] CERN, Geneva, Switzerland.
[Khubua, J.] GTU, Tbilisi, Rep of Georgia.
[Kono, T.; Nagai, R.] Ochanomizu Univ, Ochadai Acad Prod, Tokyo, Japan.
[Konoplich, R.] Manhattan Coll, New York, NY USA.
[Leisos, A.] Hellen Open Univ, Patras, Greece.
[Lin, S. C.] Acad Sinica, Inst Phys, Acad Sinica Grid Comp, Taipei, Taiwan.
[Liu, B.] Shandong Univ, Sch Phys, Jinan, Shandong, Peoples R China.
[Myagkov, A. G.; Nikolaenko, V.; Zaitsev, A. M.] Moscow Inst Phys & Technol, Dolgoprudnyi, Russia.
[Nessi, M.] Univ Geneva, Sect Phys, Geneva, Switzerland.
[Pasztor, G.] Eotvos Lorand Univ, Budapest, Hungary.
[Pinamonti, M.] SISSA, Trieste, Italy.
[Purohit, M.] Univ South Carolina, Dept Phys & Astron, Columbia, SC USA.
[Shi, L.] Sun Yat Sen Univ, Sch Phys & Engn, Guangzhou, Peoples R China.
[Shiyakova, M.] Bulgarian Acad Sci, INRNE, Sofia, Bulgaria.
[Smirnova, L. N.] Moscow MV Lomonosov State Univ, Fac Phys, Moscow, Russia.
[Sood, A.; Zhang, G.] Acad Sinica, Inst Phys, Taipei, Taiwan.
[Tikhomirov, V. O.] Natl Res Nucl Univ MEPhI, Moscow, Russia.
[Tompkins, L.] Stanford Univ, Dept Phys, Stanford, CA 94305 USA.
[Toth, J.] Wigner Res Ctr Phys, Inst Particle & Nucl Phys, Budapest, Hungary.
[Vest, A.] Flensburg Univ Appl Sci, Flensburg, Germany.
[Yusuff, I.] Univ Malaya, Dept Phys, Kuala Lumpur, Malaysia.
[Zhang, R.] Aix Marseille Univ, CPPM, Marseille, France.
[Zhang, R.] CNRS, IN2P3, Marseille, France.
PKU CHEP, Beijing, Peoples R China.
RP Aaboud, M (reprint author), Univ Mohamed Premier, Fac Sci, Oujda, Morocco.
RI Guo, Jun/O-5202-2015; Gladilin, Leonid/B-5226-2011; Villa,
Mauro/C-9883-2009; Peleganchuk, Sergey/J-6722-2014; messina,
andrea/C-2753-2013; Yang, Haijun/O-1055-2015; White, Ryan/E-2979-2015;
Li, Liang/O-1107-2015; Monzani, Simone/D-6328-2017; Warburton,
Andreas/N-8028-2013; Tikhomirov, Vladimir/M-6194-2015; Livan,
Michele/D-7531-2012; Kuday, Sinan/C-8528-2014; Doyle,
Anthony/C-5889-2009; Mitsou, Vasiliki/D-1967-2009; Solodkov,
Alexander/B-8623-2017; Camarri, Paolo/M-7979-2015; Carvalho,
Joao/M-4060-2013; Prokoshin, Fedor/E-2795-2012
OI Guo, Jun/0000-0001-8125-9433; Gladilin, Leonid/0000-0001-9422-8636;
Villa, Mauro/0000-0002-9181-8048; Peleganchuk,
Sergey/0000-0003-0907-7592; White, Ryan/0000-0003-3589-5900; Li,
Liang/0000-0001-6411-6107; Monzani, Simone/0000-0002-0479-2207;
Warburton, Andreas/0000-0002-2298-7315; Tikhomirov,
Vladimir/0000-0002-9634-0581; Livan, Michele/0000-0002-5877-0062; Kuday,
Sinan/0000-0002-0116-5494; Doyle, Anthony/0000-0001-6322-6195; Mitsou,
Vasiliki/0000-0002-1533-8886; Solodkov, Alexander/0000-0002-2737-8674;
Camarri, Paolo/0000-0002-5732-5645; Carvalho, Joao/0000-0002-3015-7821;
Prokoshin, Fedor/0000-0001-6389-5399
FU ANPCyT, Argentina; YerPhI, Armenia; ARC, Australia; BMWFW, Austria; FWF,
Austria; ANAS, Azerbaijan; SSTC, Belarus; CNPq, Brazil; FAPESP, Brazil;
NSERC, Canada; NRC, Canada; CFI, Canada; CERN; CONICYT, Chile; CAS,
China; MOST, China; NSFC, China; COLCIENCIAS, Colombia; MSMT CR, Czech
Republic; MPO CR, Czech Republic; VSC CR, Czech Republic; DNRF, Denmark;
DNSRC, Denmark; IN2P3-CNRS, France; CEA-DSM/IRFU, France; GNSF, Georgia;
BMBF, Germany; HGF, Germany; MPG, Germany; GSRT, Greece; RGC, China;
Hong Kong SAR, China; ISF, Israel; I-CORE, Israel; Benoziyo Center,
Israel; INFN, Italy; MEXT, Japan; JSPS, Japan; CNRST, Morocco; FOM,
Netherlands; NWO, Netherlands; RCN, Norway; MNiSW, Poland; NCN, Poland;
FCT, Portugal; MNE/IFA, Romania; MES of Russia, Russian Federation; NRC
KI, Russian Federation; JINR; MESTD, Serbia; MSSR, Slovakia; ARRS,
Slovenia; MIZS, Slovenia; DST/NRF, South Africa; MINECO, Spain; SRC,
Sweden; Wallenberg Foundation, Sweden; SERI, Switzerland; SNSF,
Switzerland; Canton of Bern, Switzerland; Canton of Geneva, Switzerland;
MOST, Taiwan; TAEK, Turkey; STFC, United Kingdom; DOE, United States of
America; NSF, United States of America; BCKDF, Canada; Canada Council,
Canada; CANARIE, Canada; CRC, Canada; Compute Canada, Canada; FQRNT,
Canada; Ontario Innovation Trust, Canada; EPLANET; ERC; FP7; Horizon
2020; Marie Sklodowska-Curie Actions; European Union; Investissements
d'Avenir Labex and Idex, France; ANR, France; Region Auvergne, France;
Fondation Partager le Savoir, France; DFG, Germany; AvH Foundation,
Germany; Herakleitos, Thales; Aristeia programmes; EU-ESF; Greek NSRF;
BSF, Israel; GIF, Israel; Minerva, Israel; BRF, Norway; Generalitat de
Catalunya, Spain; Generalitat Valenciana, Spain; Royal Society, United
Kingdom; Leverhulme Trust, United Kingdom
FX We acknowledge the support of ANPCyT, Argentina; YerPhI, Armenia; ARC,
Australia; BMWFW and FWF, Austria; ANAS, Azerbaijan; SSTC, Belarus; CNPq
and FAPESP, Brazil; NSERC, NRC and CFI, Canada; CERN; CONICYT, Chile;
CAS, MOST and NSFC, China; COLCIENCIAS, Colombia; MSMT CR, MPO CR and
VSC CR, Czech Republic; DNRF and DNSRC, Denmark; IN2P3-CNRS,
CEA-DSM/IRFU, France; GNSF, Georgia; BMBF, HGF, and MPG, Germany; GSRT,
Greece; RGC, Hong Kong SAR, China; ISF, I-CORE and Benoziyo Center,
Israel; INFN, Italy; MEXT and JSPS, Japan; CNRST, Morocco; FOM and NWO,
Netherlands; RCN, Norway; MNiSW and NCN, Poland; FCT, Portugal; MNE/IFA,
Romania; MES of Russia and NRC KI, Russian Federation; JINR; MESTD,
Serbia; MSSR, Slovakia; ARRS and MIZS, Slovenia; DST/NRF, South Africa;
MINECO, Spain; SRC and Wallenberg Foundation, Sweden; SERI, SNSF and
Cantons of Bern and Geneva, Switzerland; MOST, Taiwan; TAEK, Turkey;
STFC, United Kingdom; DOE and NSF, United States of America. In
addition, individual groups and members have received support from
BCKDF, the Canada Council, CANARIE, CRC, Compute Canada, FQRNT, and the
Ontario Innovation Trust, Canada; EPLANET, ERC, FP7, Horizon 2020 and
Marie Sklodowska-Curie Actions, European Union; Investissements d'Avenir
Labex and Idex, ANR, Region Auvergne and Fondation Partager le Savoir,
France; DFG and AvH Foundation, Germany; Herakleitos, Thales and
Aristeia programmes co-financed by EU-ESF and the Greek NSRF; BSF, GIF
and Minerva, Israel; BRF, Norway; Generalitat de Catalunya, Generalitat
Valenciana, Spain; the Royal Society and Leverhulme Trust, United
Kingdom.; The crucial computing support from all WLCG partners is
acknowledged gratefully, in particular from CERN and the ATLAS Tier-1
facilities at TRIUMF (Canada), NDGF (Denmark, Norway, Sweden), CC-IN2P3
(France), KIT/GridKA (Germany), INFN-CNAF (Italy), NL-T1 (Netherlands),
PIC (Spain), ASGC (Taiwan), RAL (UK) and BNL (USA) and in the Tier-2
facilities worldwide.
NR 77
TC 1
Z9 1
U1 23
U2 23
PU ELSEVIER SCIENCE BV
PI AMSTERDAM
PA PO BOX 211, 1000 AE AMSTERDAM, NETHERLANDS
SN 0370-2693
EI 1873-2445
J9 PHYS LETT B
JI Phys. Lett. B
PD OCT 10
PY 2016
VL 761
BP 350
EP 371
DI 10.1016/j.physletb.2016.08.042
PG 22
WC Astronomy & Astrophysics; Physics, Nuclear; Physics, Particles & Fields
SC Astronomy & Astrophysics; Physics
GA DX6CI
UT WOS:000384469900052
ER
PT J
AU Aaboud, M
Aad, G
Abbott, B
Abdallah, J
Abdinov, O
Abeloos, B
Aben, R
AbouZeid, OS
Abraham, NL
Abramowicz, H
Abreu, H
Abreu, R
Abulaiti, Y
Acharya, BS
Adamczyk, L
Adams, DL
Adelman, J
Adomeit, S
Adye, T
Affolder, AA
Agatonovic-Jovin, T
Agricola, J
Aguilar-Saavedra, JA
Ahlen, SP
Ahmadov, F
Aielli, G
Akerstedt, H
Akesson, TPA
Akimov, AV
Alberghi, GL
Albert, J
Albrand, S
Verzini, MJA
Aleksa, M
Aleksandrov, IN
Alexa, C
Alexander, G
Alexopoulos, T
Alhroob, M
Ali, B
Aliev, M
Alimonti, G
Alison, J
Alkire, SP
Allbrooke, BMM
Allen, BW
Allport, PP
Aloisio, A
Alonso, A
Alonso, F
Alpigiani, C
Alstaty, M
Gonzalez, BA
Piqueras, DA
Alviggi, MG
Amadio, BT
Amako, K
Coutinho, YA
Amelung, C
Amidei, D
Dos Santos, SPA
Amorim, A
Amoroso, S
Amundsen, G
Anastopoulos, C
Ancu, LS
Andari, N
Andeen, T
Anders, CF
Anders, G
Anders, JK
Anderson, KJ
Andreazza, A
Andrei, V
Angelidakis, S
Angelozzi, I
Anger, P
Angerami, A
Anghinolfi, F
Anisenkov, AV
Anjos, N
Annovi, A
Antel, C
Antonelli, M
Antonov, A
Anulli, F
Aoki, M
Bella, LA
Arabidze, G
Arai, Y
Araque, JP
Arce, ATH
Arduh, FA
Arguin, JF
Argyropoulos, S
Arik, M
Armbruster, AJ
Armitage, LJ
Arnaez, O
Arnold, H
Arratia, M
Arslan, O
Artamonov, A
Artoni, G
Artz, S
Asai, S
Asbah, N
Ashkenazi, A
Asman, B
Asquith, L
Assamagan, K
Astalos, R
Atkinson, M
Atlay, NB
Augsten, K
Avolio, G
Axen, B
Ayoub, MK
Azuelos, G
Baak, MA
Baas, AE
Baca, MJ
Bachacou, H
Bachas, K
Backes, M
Backhaus, M
Bagiacchi, P
Bagnaia, P
Bai, Y
Baines, JT
Baker, OK
Baldin, EM
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Zhao, Y.
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Zhou, L.
Zhou, M.
Zhou, N.
Zhu, C. G.
Zhu, H.
Zhu, J.
Zhu, Y.
Zhuang, X.
Zhukov, K.
Zibell, A.
Zieminska, D.
Zimine, N. I.
Zimmermann, C.
Zimmermann, S.
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CA ATLAS Collaboration
TI Search for high-mass new phenomena in the dilepton final state using
proton-proton collisions at root s=13 TeV with the ATLAS detector
SO PHYSICS LETTERS B
LA English
DT Article
ID PARTON DISTRIBUTIONS; CROSS-SECTION; GAUGE BOSONS; PLUS PLUS; PHYSICS;
LHC
AB A search is conducted for both resonant and non-resonant high-mass new phenomena in dielectron and dimuon final states. The search uses 3.2 fb(-1) of proton-proton collision data, collected at root s = 13 TeV by the ATLAS experiment at the LHC in 2015. The dilepton invariant mass is used as the discriminating variable. No significant deviation from the Standard Model prediction is observed; therefore limits are set on the signal model parameters of interest at 95% credibility level. Upper limits are set on the cross-section times branching ratio for resonances decaying to dileptons, and the limits are converted into lower limits on the resonance mass, ranging between 2.74 TeV and 3.36 TeV, depending on the model. Lower limits on the llqq contact interaction scale are set between 16.7 TeV and 25.2 TeV, also depending on the model. (C) 2016 The Author. Published by Elsevier B.V.
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[Bouffard, J.; Ernst, J.; Fischer, A.; Guindon, S.; Jain, V.] SUNY Albany, Dept Phys, Albany, NY 12222 USA.
[Czodrowski, P.; Dassoulas, J.; Dehghanian, N.; Gingrich, D. M.; Jabbar, S.; Karamaoun, A.; Moore, R. W.; Pinfold, J. L.] Univ Alberta, Dept Phys, Edmonton, AB, Canada.
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[Kuday, S.] CNRS, IN2P3, LAPP, Annecy Le Vieux, France.
[Blair, R. E.; Chekanov, S.; LeCompte, T.; Love, J.; Malon, D.; Metcalfe, J.; Nguyen, D. H.; Nodulman, L.; Paramonov, A.; Price, L. E.; Proudfoot, J.; Ryu, S.; Stanek, R. W.; van Gemmeren, R.; Wang, R.; Webster, J. S.; Yoshida, R.; Zhang, J.] Argonne Natl Lab, Div High Energy Phys, Argonne, IL 60439 USA.
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[Brandt, A.; Bullock, D.; Darmora, S.; De, K.; Farbin, A.; Feremenga, L.; Griffiths, J.; Hadavand, H. K.; Heelan, L.; Kim, H. Y.; Ozturk, N.; Schovancova, J.; Stradling, A. R.; Usai, G.; Vartapetian, A.; White, A.; Yu, J.] Univ Texas Arlington, Dept Phys, POB 19059, Arlington, TX 76019 USA.
[Angelidakis, S.; Chouridou, S.; Fassouliotis, D.; Giokaris, N.; Ioannou, R.; Kourkoumelis, C.; Tsirintanis, N.] Univ Athens, Dept Phys, Athens, Greece.
[Alexopoulos, T.; Benekos, N.; Dris, M.; Gazis, E. N.; Karakostas, K.; Karastathis, N.; Karentzos, E.; Leontsinis, S.; Maltezos, S.; Ntekas, K.; St Panagiotopoulou, E.; Papadopoulou, Th. D.; Tsipolitis, G.; Vlachos, S.] Natl Tech Univ Athens, Dept Phys, Zografos, Greece.
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[Aleksa, M.; Gonzalez, B. Alvarez; Amoroso, S.; Anders, G.; Anghinolfi, F.; Arnaez, O.; Avolio, G.; Baak, M. A.; Backes, M.; Backhaus, M.; Barak, L.; Beermann, T. A.; Beltramello, O.; Bianco, M.; Bogaerts, J. A.; Bortfeldt, J.; Boveia, A.; Boyd, J.; Burckhart, H.; Camarda, S.; Campana, S.; Garrido, M. D. M. Capeans; Carli, T.; Carrillo-Montoya, G. D.; Catinaccio, A.; Cattai, A.; Cerv, M.; Chromek-Burckhart, D.; Colombo, T.; Conti, G.; Dell'Acqua, A.; Deviveiros, P. O.; Di Girolamo, A.; Di Girolamo, B.; Di Nardo, R.; Dittus, F.; Dobos, D.; Dudarev, A.; Duhrssen, M.; Eifert, T.; Ellis, N.; Elsing, M.; Farthouat, P.; Fassnacht, P.; Feng, E. J.; Francis, D.; Fressard-Batraneanu, S. M.; Froidevaux, D.; Gadatsch, S.; Goossens, L.; Gorini, B.; Gray, H. M.; Gumpert, C.; Hanisch, S.; Hawkings, R. J.; Helsens, C.; Correia, A. M. Henriques; Hervas, L.; Hoecker, A.; Huhtinen, M.; Iengo, R.; Jakobsen, S.; Klioutchnikova, T.; Krasznahorkay, A.; Lapoire, C.; Lassnig, M.; Miotto, G. Lehmann; Lenzi, B.; Lichard, P.; Malyukov, S.; Mandelli, B.; Manousos, A.; Mapelli, L.; Marzin, A.; Berlingen, J. Montejo; Mornacchi, G.; Nairz, A. M.; Nakahama, Y.; Nessi, M.; Nordberg, M.; Oide, H.; Palestini, S.; Pauly, T.; Pernegger, H.; Petersen, B. A.; Pommes, K.; Poppleton, A.; Poulard, G.; Poveda, J.; Astigarraga, M. E. Pozo; Rammensee, M.; Raymond, M.; Rembser, C.; Ritsch, E.; Roe, S.; Ruthmann, N.; Salzburger, A.; Schaefer, D.; Schlenker, S.; Schmieden, K.; Sforza, F.; Sanchez, C. A. Solans; Spigo, G.; Starz, S.; Stelzer, H. J.; Teischinger, Ea.; Ten Kate, H.; Unal, G.; van Woerden, M. C.; Vandelli, W.; Voss, R.; Vuillermet, R.; Wells, P. S.; Wengler, T.; Wenig, S.; Werner, R.; Wilkens, H. G.; Wotschack, J.; Young, C. J. S.; Zwalinski, L.] CERN, Geneva, Switzerland.
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[Blunier, S.; Diaz, M. A.; Ochoa-Ricoux, J. P.] Pontificia Univ Catolica Chile, Dept Fis, Santiago, Chile.
[Brooks, W. K.; Carquin, E.; Kuleshov, S.; Pezoa, R.; Prokoshin, F.; Loyola, J. E. Salazar; Araya, S. Tapia; White, R.] Univ Tecn Federico Santa Maria, Dept Fis, Valparaiso, Chile.
[Bai, Y.; da Costa, J. Barreiro Guimaraes; Cheng, H. J.; Fang, Y.; Jin, S.; Li, Q.; Liang, Z.; Merino, J. Llorente; Lou, X.; Mansour, J. D.; Ouyang, Q.; Peng, C.; Ren, H.; Shan, L. Y.; Sun, X.; Xu, D.; Zhu, H.; Zhuang, X.] Chinese Acad Sci, Inst High Energy Phys, Beijing, Peoples R China.
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[Boumediene, D.; Busato, E.; Calvet, D.; Calvet, S.; Chomont, A. R.; Donini, J.; Gris, Ph.; Madar, R.; Pallin, D.; Saez, S. M. Romano; Santoni, C.; Simon, D.; Vazeille, F.] Univ Blaise Pascal, Clermont Ferrand, France.
[Boumediene, D.; Busato, E.; Calvet, D.; Calvet, S.; Chomont, A. R.; Donini, J.; Gris, Ph.; Madar, R.; Pallin, D.; Saez, S. M. Romano; Santoni, C.; Simon, D.; Vazeille, F.] CNRS, IN2P3, Clermont Ferrand, France.
[Alkire, S. P.; Angerami, A.; Brooijmans, G.; Carbone, R. M.; Clark, M. R.; Cole, B.; Hu, D.; Hughes, E. W.; Iordanidou, K.; Klein, M. H.; Mohapatra, S.; Ochoa, I.; Parsons, J. A.; Smith, M. N. K.; Smith, R. W.; Thompson, E. N.; Tuts, P. M.; Wang, T.; Zhou, L.] Columbia Univ, Nevis Lab, Irvington, NY USA.
[Alonso, A.; Besjes, G. J.; Dam, M.; Galster, G.; Hansen, J. B.; Hansen, J. D.; Hansen, P. H.; Loevschall-Jensen, A. E.; Monk, J.; Mortensen, S. S.; Pedersen, L. E.; Petersen, T. C.; Pingel, A.; Wiglesworth, C.; Xella, S.] Univ Copenhagen, Niels Bohr Inst, Copenhagen, Denmark.
[Cairo, V. M.; Capua, M.; Crosetti, G.; Del Gaudio, M.; La Rotonda, L.; Mastroberardino, A.; Policicchio, A.; Salvatore, D.; Scarfone, V.; Schioppa, M.; Susinno, G.; Tassi, E.] Ist Nazl Fis Nucl, Lab Nazl Frascati, Grp Collegato Cosenza, Frascati, Italy.
[Cairo, V. M.; Capua, M.; Crosetti, G.; Del Gaudio, M.; La Rotonda, L.; Mastroberardino, A.; Policicchio, A.; Salvatore, D.; Scarfone, V.; Schioppa, M.; Susinno, G.; Tassi, E.] Univ Calabria, Dipartimento Fis, Arcavacata Di Rende, Italy.
[Adamczyk, L.; Bold, T.; Dabrowski, W.; Gach, G. P.; Grabowska-Bold, I.; Kisielewska, D.; Koperny, S.; Kowalski, T. Z.; Mindur, B.; Przybycien, M.; Zemla, A.] AGH Univ Sci & Technol, Fac Phys & Appl Comp Sci, Krakow, Poland.
[Banas, E.; de Renstrom, P. A. Bruckman; Burka, K.; Chwastowski, J. J.; Derendarz, D.; Godlewski, J.; Gornicki, E.; Hajduk, Z.; Iwanski, W.; Kaczmarska, A.; Knapik, J.; Korcyl, K.; Kowalewska, A. B.; Malecki, Pa.; Olszewski, A.; Olszowska, J.; Stanecka, E.; Staszewski, R.; Trzebinski, M.; Trzupek, A.; Wolter, M. W.; Wosiek, B. K.; Wozniak, K. W.; Zabinski, B.] Polish Acad Sci, Inst Nucl Phys, Krakow, Poland.
[Cao, T.; Firan, A.; Hetherly, J. W.; Kama, S.; Kehoe, R.; Sekula, S. J.; Stroynowski, R.; Turvey, A. J.; Varol, T.; Wang, H.; Ye, J.; Zhao, X.; Zhou, L.] Southern Methodist Univ, Dept Phys, Dallas, TX USA.
[Izen, J. M.; Leyton, M.; Meirose, B.; Namasivayam, H.; Reeves, K.] Univ Texas Dallas, Dept Phys, Richardson, TX 75083 USA.
[Asbah, N.; Behr, J. K.; Bertsche, C.; Bessner, M.; Bloch, I.; Britzger, D.; Deterre, C.; Dutta, B.; Dyndal, M.; Eckardt, C.; Filipuzzi, M.; Flaschel, N.; Bravo, A. Gascon; Glazov, A.; Gregor, I. M.; Haleem, M.; Hamnett, P. G.; Hiller, K. H.; Howarth, J.; Huang, Y.; Katzy, J.; Keller, J. S.; Kondrashova, N.; Kuhl, T.; Lobodzinska, E.; Lohwasser, K.; Madsen, A.; Medinnis, M.; Monig, K.; Garcia, R. F. Naranjo; Naumann, T.; O'Rourke, A. A.; Peschke, R.; Peters, K.; Pirumov, H.; Poley, A.; Robinson, J. E. M.; Schaefer, R.; Schmitt, S.; South, D.; Stanescu-Bellu, M.; Stanitzki, M. M.; Styles, N. A.; Tackmann, K.; Trofymov, A.; Wang, J.; Zakharchuk, N.] DESY, Hamburg, Germany.
[Asbah, N.; Behr, J. K.; Bertsche, C.; Bessner, M.; Bloch, I.; Britzger, D.; Deterre, C.; Dutta, B.; Dyndal, M.; Eckardt, C.; Filipuzzi, M.; Flaschel, N.; Bravo, A. Gascon; Glazov, A.; Gregor, I. M.; Haleem, M.; Hamnett, P. G.; Hiller, K. H.; Howarth, J.; Huang, Y.; Katzy, J.; Keller, J. S.; Kondrashova, N.; Kuhl, T.; Lobodzinska, E.; Lohwasser, K.; Madsen, A.; Medinnis, M.; Monig, K.; Garcia, R. F. Naranjo; Naumann, T.; O'Rourke, A. A.; Peschke, R.; Peters, K.; Pirumov, H.; Poley, A.; Robinson, J. E. M.; Schaefer, R.; Schmitt, S.; South, D.; Stanescu-Bellu, M.; Stanitzki, M. M.; Styles, N. A.; Tackmann, K.; Trofymov, A.; Wang, J.; Zakharchuk, N.] DESY, Zeuthen, Germany.
[Burmeister, I.; Cinca, D.; Dette, K.; Erdmann, J.; Esch, H.; Gossling, C.; Homann, M.; Jentzsch, J.; Klingenberg, R.; Kroeninger, K.] Tech Univ Dortmund, Inst Expt Phys 4, Dortmund, Germany.
[Anger, P.; Duschinger, D.; Friedrich, F.; Grohs, J. P.; Gutschow, C.; Hauswald, L.; Kobel, M.; Mader, W. F.; Novgorodova, O.; Siegert, F.; Socher, F.; Straessner, A.; Vest, A.; Wahrmund, S.] Tech Univ Dresden, Inst Kern & Teilchenphys, Dresden, Germany.
[Arce, A. T. H.; Benjamin, D. P.; Bjergaard, D. M.; Bocci, A.; Cerio, B. C.; Goshaw, A. T.; Kajomovitz, E.; Kotwal, A.; Kruse, M. C.; Li, L.; Li, S.; Liu, M.; Oh, S. H.; Zhou, C.] Duke Univ, Dept Phys, Durham, NC 27706 USA.
[Bristow, T. M.; Clark, P. J.; Dias, F. A.; Edwards, N. C.; Gao, Y.; Walls, F. M. Garay; Glaysher, P. C. F.; Harrington, R. D.; Leonidopoulos, C.; Martin, V. J.; Mills, C.; Pino, S. A. Olivares; Proissl, M.; Washbrook, A.; Wynne, B. M.] Univ Edinburgh, SUPA Sch Phys & Astron, Edinburgh, Midlothian, Scotland.
[Antonelli, M.; Beretta, M.; Bilokon, H.; Chiarella, V.; Curatolo, M.; Esposito, B.; Gatti, C.; Laurelli, R.; Maccarrone, G.; Mancini, G.; Santoni, A.; Testa, M.; Vilucchi, E.] Ist Nazl Fis Nucl, Lab Nazl Frascati, Frascati, Italy.
[Arnold, H.; Betancourt, C.; Boehler, M.; Bruneliere, R.; Buehrer, F.; Burgard, C. D.; Buescher, D.; Cardillo, F.; Coniavitis, E.; Consorti, V.; Dang, N. P.; Dao, V.; Di Simone, A.; Glatzer, J.; Gonella, G.; Herten, G.; Hirose, M.; Jakobs, K.; Javurek, T.; Jenni, R.; Kiss, F.; Koneke, K.; Kopp, A. K.; Kuehn, S.; Landgraf, U.; Luedtke, C.; Nagel, M.; Pagacova, M.; Parzefall, U.; Ronzani, M.; Rosbach, K.; Ruhr, F.; Rurikova, Z.; Sammel, D.; Schillo, C.; Schnoor, U.; Schumacher, M.; Sommer, R.; Sundermann, J. E.; Ta, D.; Temming, K. K.; Tsiskaridze, V.; Weiser, C.; Werner, M.; Zhang, L.; Zimmermann, S.] Albert Ludwigs Univ, Fak Math & Phys, Freiburg, Germany.
[Ancu, L. S.; De Mendizabal, J. Bilbao; Calace, N.; Chatterjee, A.; Clark, A.; Coccaro, A.; Delitzsch, C. M.; della Volpe, D.; Ferrere, D.; Gadomski, S.; Golling, T.; Gonzalez-Sevilla, S.; Gramling, J.; Guescini, F.; Iacobucci, G.; Katre, A.; Khoo, T. J.; Lionti, A. E.; March, L.; Mermod, R.; Miucci, A.; Nackenhorst, O.; Paolozzi, L.; Ristic, B.; Schramm, S.; Sfyrla, A.; Vallecorsa, S.; Wu, X.] Univ Geneva, Sect Phys, Geneva, Switzerland.
[Barberis, D.; Darbo, G.; Favareto, A.; Parodi, A. Ferretto; Gagliardi, G.; Gaudiello, A.; Gemme, C.; Guido, E.; Miglioranzi, S.; Morettini, R.; Osculati, B.; Parodi, F.; Passaggio, S.; Rossi, L. P.; Sannino, M.; Schiavi, C.] Ist Nazl Fis Nucl, Sez Genova, Genoa, Italy.
[Barberis, D.; Favareto, A.; Parodi, A. Ferretto; Gagliardi, G.; Gaudiello, A.; Guido, E.; Miglioranzi, S.; Osculati, B.; Parodi, F.; Sannino, M.; Schiavi, C.] Univ Genoa, Dipartimento Fis, Genoa, Italy.
[Jejelava, J.; Tskhadadze, E. G.] Iv Javakhishvili Tbilisi State Univ, E Andronikashvili Inst Phys, Tbilisi, Rep of Georgia.
[Djobava, T.; Durglishvili, A.; Khubua, J.; Mosidze, M.] Tbilisi State Univ, Inst High Energy Phys, Tbilisi, Rep of Georgia.
[Duren, M.; Heinz, C.; Kreutzfeldt, K.; Stenzel, H.] Justus Liebig Univ Giessen, Inst Phys 2, Giessen, Germany.
[Bates, R. L.; Boutle, S. K.; Madden, W. D. Breaden; Britton, D.; Buckley, A. G.; Bussey, P.; Buttar, C. M.; Buzatu, A.; Crawley, S. J.; D'Auria, S.; Doyle, A. T.; Ferrando, J.; Gul, U.; Knue, A.; Mullen, R.; O'Shea, V.; Owen, M.; Pollard, C. S.; Qin, G.; Quilty, D.; Ravenscroft, T.; Robson, A.; St Denis, R. D.; Stewart, G. A.; Thompson, A. S.] Univ Glasgow, SUPA Sch Phys & Astron, Glasgow, Lanark, Scotland.
[Agricola, J.; Bindi, M.; Blumenschein, U.; Brandt, G.; De Maria, A.; Drechsler, E.; Graber, L.; Grosse-Knetter, J.; Janus, M.; Kareem, M. J.; Kawamura, G.; Lai, S.; Lemmer, B.; Magradze, E.; Mantoani, M.; Mchedlidze, G.; Llacer, M. Moreno; Musheghyan, H.; Quadt, A.; Rieger, J.; Rosien, N-A.; Rzehorz, G. F.; Shabalina, E.; Stolte, R.; Veatch, J.; Weingarten, J.; Zinonos, Z.] Georg August Univ, Inst Phys 2, Gottingen, Germany.
[Albrand, S.; Berlendis, S.; Camincher, C.; Collot, J.; Crepe-Renaudin, S.; Delsart, P. A.; Gabaldon, C.; Genest, M. H.; Gradin, P. O. J.; Hostachy, J-Y; Ledroit-Guillon, F.; Lleres, A.; Lucotte, A.; Malek, F.; Petit, E.; Stark, J.; Trocme, B.; Wu, M.] Univ Grenoble Alpes, CNRS, IN2P3, Lab Phys Subat & Cosmol, Grenoble, France.
[McFarlane, K. W.] Hampton Univ, Dept Phys, Hampton, VA 23668 USA.
[Chan, S. K.; Clark, B. L.; Franklin, M.; Giromini, P.; Huth, J.; Ippolito, V.; Lazovich, T.; Mateos, D. Lopez; Morii, M.; Rogan, C. S.; Skottowe, H. P.; Sun, S.; Tolley, E.; Tong, B.; Tuna, A. N.; Yen, A. L.; Zambito, S.] Harvard Univ, Lab Particle Phys & Cosmol, Cambridge, MA USA.
[Andrei, V.; Antel, C.; Baas, A. E.; Brandt, O.; Djuvsland, J. I.; Dunford, M.; Geisler, M. P.; Hanke, R.; Jongmanns, J.; Kluge, E. -E.; Lang, V. S.; Meier, K.; Zu Theenhausen, H. Meyer; Villar, D. I. Narrias; Sahinsoy, M.; Scharf, V.; Schultz-Coulon, H-C.; Stamen, R.; Starovoitov, R.; Suchek, S.; Wessels, M.] Heidelberg Univ, Kirchhoff Inst Phys, Heidelberg, Germany.
[Anders, C. F.; de Lima, D. E. Ferreira; Giulini, M.; Kolb, M.; Lisovyi, M.; Radescu, V.; Schaetzel, S.; Schoening, A.; Sosa, D.] Heidelberg Univ, Inst Phys, Heidelberg, Germany.
[Nagasaka, Y.] Hiroshima Inst Technol, Fac Appl Informat Sci, Hiroshima, Japan.
[Bortolotto, V.; Chan, Y. L.; Castillo, L. R. Flores; Lu, H.; Salvucci, A.; Tsui, K. M.] Chinese Univ Hong Kong, Dept Phys, Shatin, Hong Kong, Peoples R China.
[Bortolotto, V.; Orlando, N.] Univ Hong Kong, Dept Phys, Hong Kong, Hong Kong, Peoples R China.
[Bortolotto, V.; Prokofiev, K.] Hong Kong Univ Sci & Technol, Dept Phys, Kowloon, Hong Kong, Peoples R China.
[Choi, K.; Dattagupta, A.; Evans, H.; Gagnon, P.; Kopeliansky, R.; Lammers, S.; Martinez, N. Lorenzo; Luehring, F.; Ogren, H.; Penwell, J.; Weinert, B.; Zieminska, D.] Indiana Univ, Dept Phys, Bloomington, IN 47405 USA.
[Guenther, J.; Jansky, R.; Kneringer, E.; Lukas, W.; Milic, A.; Usanova, A.; Vigne, R.] Leopold Franzens Univ, Inst Astro & Teilchenphys, Innsbruck, Austria.
[Abdallah, J.; Argyropoulos, S.; Benitez, J.; Mallik, U.] Univ Iowa, Iowa City, IA USA.
[Chen, C.; Cochran, J.; De Lorenzi, F.; Jiang, H.; Krumnack, N.; Pluth, D.; Prell, S.; Werner, M. D.; Yu, J.] Iowa State Univ, Dept Phys & Astron, Ames, IA USA.
[Ahmadov, F.; Aleksandrov, I. N.; Bednyakov, V. A.; Boyko, I. R.; Budagov, I. A.; Chelkov, G. A.; Cheplakov, A.; Chizhov, M. V.; Dedovich, D. V.; Demichev, M.; Gongadze, A.; Gostkin, M. I.; Huseynov, N.; Javadov, N.; Karpov, S. N.; Karpova, Z. M.; Khramov, E.; Kruchonak, U.; Kukhtin, V.; Ladygin, E.; Lyubushkin, V.; Minashvili, I. A.; Mineev, M.; Peshekhonov, V. D.; Plotnikova, E.; Potrap, I. N.; Pozdnyakov, V.; Rusakovich, N. A.; Sadykov, R.; Sapronov, A.; Shiyakova, M.; Soloshenko, A.; Vinogradov, V. B.; Yeletskikh, I.; Zhemchugov, A.; Zimine, N. I.] JINR Dubna, Dubna, Russia.
[Amako, K.; Aoki, M.; Arai, Y.; Hanagaki, K.; Ikegami, Y.; Ikeno, M.; Iwasaki, H.; Kanzaki, J.; Kondo, T.; Kono, T.; Makida, Y.; Nagai, R.; Nagano, K.; Nakamura, K.; Nozaki, M.; Odaka, S.; Okuyama, T.; Sasaki, O.; Suzuki, S.; Takubo, Y.; Tanaka, S.; Terada, S.; Tokushuku, K.; Tsuno, S.; Unno, Y.; Yamamoto, A.; Yasu, Y.] KEK, High Energy Accelerator Res Org, Tsukuba, Ibaraki, Japan.
[Chen, Y.; Hasegawa, M.; Kido, S.; Kishimoto, T.; Kurashige, H.; Maeda, J.; Ochi, A.; Shimizu, S.; Yakabe, R.; Yamazaki, Y.; Yuan, L.] Kobe Univ, Grad Sch Sci, Kobe, Hyogo, Japan.
[Ishino, M.; Kunigo, T.; Monden, R.; Sumida, T.; Tashiro, T.] Kyoto Univ, Fac Sci, Kyoto, Japan.
[Stamm, S.; Takashima, R.] Kyoto Univ, Kyoto, Japan.
[Kawagoe, K.; Oda, S.; Otono, H.; Tojo, J.] Kyushu Univ, Dept Phys, Fukuoka, Japan.
[Alconada Verzini, M. J.; Alonso, F.; Arduh, F. A.; Dova, M. T.; Monticelli, F.; Wahlberg, H.] Univ Nacl La Plata, Inst Fis La Plata, La Plata, Buenos Aires, Argentina.
[Alconada Verzini, M. J.; Alonso, F.; Arduh, F. A.; Dova, M. T.; Monticelli, F.; Wahlberg, H.] Consejo Nacl Invest Cient & Tecn, La Plata, Buenos Aires, Argentina.
[Barton, A. E.; Beattie, M. D.; Bertram, I. A.; Borissov, G.; Bouhova-Thacker, E. V.; Cheatham, S.; Dearnaley, W. J.; Fox, H.; Grimm, K.; Henderson, R. C. W.; Hughes, G.; Jones, R. W. L.; Kartvelishvili, V.; Long, R. E.; Love, P. A.; Muenstermann, D.; Parker, A. J.; Skinner, M. B.; Smizanska, M.; Walder, J.; Wharton, A. M.] Univ Lancaster, Dept Phys, Lancaster, England.
[Aliev, M.; Bachas, K.; Chiodini, G.; Gorini, E.; Longo, L.; Primavera, M.; Reale, M.; Spagnolo, S.; Ventura, A.] Ist Nazl Fis Nucl, Sez Lecce, Lecce, Italy.
[Aliev, M.; Bachas, K.; Gorini, E.; Longo, L.; Reale, M.; Spagnolo, S.; Ventura, A.] Univ Salento, Dipartimento Matemat & Fis, Lecce, Italy.
[Affolder, A. A.; D'Onofrio, M.] Univ Liverpool, Oliver Lodge Lab, Liverpool, Merseyside, England.
[Cindro, V.; Deliyergiyev, M.; Filipcic, A.; Gorisek, A.; Kanjir, L.; Kersevan, B. P.; Kramberger, G.; Macek, B.; Mandic, I.; Mikuz, M.; Muskinja, M.; Sfiligoj, T.; Sokhrannyi, G.] Jozef Stefan Inst, Dept Phys, Ljubljana, Slovenia.
[Cindro, V.; Deliyergiyev, M.; Filipcic, A.; Gorisek, A.; Kanjir, L.; Kersevan, B. P.; Kramberger, G.; Macek, B.; Mandic, I.; Mikuz, M.; Muskinja, M.; Sfiligoj, T.; Sokhrannyi, G.] Univ Ljubljana, Ljubljana, Slovenia.
[Armitage, L. J.; Bevan, A. J.; Bona, M.; Cerrito, L.; Hays, J. M.; Hickling, R.; Landon, M. P. J.; Lewis, D.; Lloyd, S. L.; Morris, J. D.; Nooney, T.; Piccaro, E.; Rizvi, E.; Sandbach, R. L.] Queen Mary Univ London, Sch Phys & Astron, London, England.
[Berry, T.; Blanco, J. E.; Boisvert, V.; Brooks, T.; Connelly, I. A.; Cowan, G.; Duguid, L.; Giannelli, M. Faucci; George, S.; Gibson, S. M.; Kempster, J. J.; Vazquez, J. G. Panduro; Pastore, Fr.; Savage, G.; Sowden, B. C.; Spano, F.; Teixeira-Dias, R.; Thomas-Wilsker, J.] Royal Holloway Univ London, Dept Phys, Surrey, England.
[Bell, A. S.; Butterworth, J. M.; Campanelli, M.; Christodoulou, V.; Cooper, B. D.; Davison, P.; Falla, R. J.; Freeborn, D.; Gregersen, K.; Ortiz, N. G. Gutierrez; Hesketh, G. G.; Jansen, E.; Jiggins, S.; Konstantinidis, N.; Korn, A.; Kucuk, H.; Leney, K. J. C.; Martyniuk, A. C.; McClymont, L. I.; Mcfayden, J. A.; Nurses, E.; Richter, S.; Scanlon, T.; Sherwood, R.; Simmons, B.; Wardrope, D. R.; Waugh, B. M.] UCL, Dept Phys & Astron, London, England.
[Greenwood, Z. D.; Grossi, G. C.; Jana, D. K.; Sawyer, L.; Subramaniam, R.] Louisiana Tech Univ, Ruston, LA 71270 USA.
[Beau, T.; Bomben, M.; Calderini, G.; Crescioli, F.; De Cecco, S.; Demilly, A.; Derue, F.; Francavilla, P.; Krasny, M. W.; Lacour, D.; Laforge, B.; Laplace, S.; Le Dortz, O.; Lefebvre, G.; Solis, A. Lopez; Luzi, P. M.; Malaescu, B.; Marchiori, G.; Nikolic-Audit, I.; Ocariz, J.; Pandini, C. E.; Pires, S.; Ridel, M.; Roos, L.; Trincaz-Duvoid, S.; Varouchas, D.; Yap, Y. C.] UPMC, Lab Phys Nucl & Hautes Energies, Paris, France.
[Beau, T.; Bomben, M.; Calderini, G.; Crescioli, F.; De Cecco, S.; Demilly, A.; Derue, F.; Francavilla, P.; Krasny, M. W.; Lacour, D.; Laforge, B.; Laplace, S.; Le Dortz, O.; Lefebvre, G.; Solis, A. Lopez; Luzi, P. M.; Malaescu, B.; Marchiori, G.; Nikolic-Audit, I.; Ocariz, J.; Pandini, C. E.; Pires, S.; Ridel, M.; Roos, L.; Trincaz-Duvoid, S.; Varouchas, D.; Yap, Y. C.] Univ Paris Diderot, Paris, France.
[Beau, T.; Bomben, M.; Calderini, G.; Crescioli, F.; De Cecco, S.; Demilly, A.; Derue, F.; Francavilla, P.; Krasny, M. W.; Lacour, D.; Laforge, B.; Laplace, S.; Le Dortz, O.; Lefebvre, G.; Solis, A. Lopez; Luzi, P. M.; Malaescu, B.; Marchiori, G.; Nikolic-Audit, I.; Ocariz, J.; Pandini, C. E.; Pires, S.; Ridel, M.; Roos, L.; Trincaz-Duvoid, S.; Varouchas, D.; Yap, Y. C.] CNRS, IN2P3, Paris, France.
[Akesson, T. P. A.; Bocchetta, S. S.; Bryngemark, L.; Doglioni, C.; Floderus, A.; Hedberg, V.; Jarlskog, G.; Lytken, E.; Mjornmark, J. U.; Smirnova, O.; Viazlo, O.] Lund Univ, Inst Fys, Lund, Sweden.
[Barreiro, F.; Calvente Lopez, S.; De la Torre, H.; Del Peso, J.; Glasman, C.; Terron, J.] Univ Autonoma Madrid, Dept Fis Teor C15, Madrid, Spain.
[Artz, S.; Becker, M.; Bertella, C.; Blum, W.; Buescher, V.; Caputo, R.; Caudron, J.; Cuth, J.; Endner, O. C.; Ertel, E.; Fiedler, F.; Fullana Torregrosa, E.; Geisen, M.; Groh, S.; Heck, T.; Herr, H.; Jakobi, K. B.; Kaluza, A.; Karnevskiy, M.; Kleinknecht, K.; Kopke, L.; Lin, T. H.; Masetti, L.; Mattmann, J.; Meyer, C.; Moritz, S.; Pleskot, V.; Rave, S.; Sander, H. G.; Schaeffer, J.; Schafer, U.; Schmitt, C.; Schmitz, S.; Schott, M.; Schuh, N.; Schulte, A.; Simioni, E.; Simon, M.; Tapprogge, S.; Urrejola, R.; Webb, S.; Yildirim, E.; Zimmermann, C.; Zinser, M.] Johannes Gutenberg Univ Mainz, Inst Phys, Mainz, Germany.
[Barnes, S. L.; Bielski, R.; Cox, B. E.; Da Via, C.; Dann, N. S.; Forcolin, G. T.; Forti, A.; Ponce, J. M. Iturbe; Li, X.; Loebinger, F. K.; Marsden, S. P.; Masik, J.; Sanchez, F. J. Munoz; Neep, T. J.; Oh, A.; Ospanov, R.; Pater, J. R.; Peters, R. F. Y.; Pilkington, A. D.; Pin, A. W. J.; Price, D.; Qin, Y.; Queitsch-Maitland, M.; Raine, J. A.; Schweiger, H.; Shaw, S. M.; Tomlinson, L.; Watts, S.; Wilk, F.; Woudstra, M. J.; Wyatt, T. R.] Univ Manchester, Sch Phys & Astron, Manchester, Lancs, England.
[Aad, G.; Alstaty, M.; Barbero, M.; Calandri, A.; Calvet, T. P.; Coadou, Y.; Diaconu, C.; Diglio, S.; Djama, F.; Ellajosyula, V.; Feligioni, L.; Gao, J.; Hadef, A.; Hallewell, G. D.; Hubaut, F.; Kahn, S. J.; Knoops, E. B. F. G.; Le Guirriec, E.; Liu, J.; Liul, K.; Madaffari, D.; Monnier, E.; Muanza, S.; Nagy, E.; Pralavorio, R.; Rodina, Y.; Rozanov, A.; Talby, M.; Theveneaux-Pelzer, T.; Torres, R. E. Ticse; Tisserant, S.; Toth, J.; Touchard, F.; Vacavant, L.; Wang, C.] Aix Marseille Univ, CPPM, Marseille, France.
[Aad, G.; Alstaty, M.; Barbero, M.; Calandri, A.; Calvet, T. P.; Coadou, Y.; Diaconu, C.; Diglio, S.; Djama, F.; Ellajosyula, V.; Feligioni, L.; Gao, J.; Hadef, A.; Hallewell, G. D.; Hubaut, F.; Kahn, S. J.; Knoops, E. B. F. G.; Le Guirriec, E.; Liu, J.; Liul, K.; Madaffari, D.; Monnier, E.; Muanza, S.; Nagy, E.; Pralavorio, R.; Rodina, Y.; Rozanov, A.; Talby, M.; Theveneaux-Pelzer, T.; Torres, R. E. Ticse; Tisserant, S.; Toth, J.; Touchard, F.; Vacavant, L.; Wang, C.] CNRS, IN2P3, Marseille, France.
[Bellomo, M.; Bernard, N. R.; Brau, B.; Dallapiccola, C.; Daya-Ishmukhametova, R. K.; Moyse, E. J. W.; Pais, P.; Pettersson, N. E.; Picazio, A.; Willocq, S.] Univ Massachusetts, Dept Phys, Amherst, MA USA.
[Belanger-Champagne, C.; Chuinard, A. J.; Corriveau, F.; Keyes, R. A.; Mantifel, R.; Prince, S.; Robertson, S. H.; Robichaud-Veronneau, A.; Stockton, M. C.; Stoebe, M.; Vachon, B.; Schroeder, T. Vazquez; Wang, K.; Warburton, A.] McGill Univ, Dept Phys, Montreal, PQ, Canada.
[Barberio, E. L.; Brennan, A. J.; Dawe, E.; Goldfarb, S.; Jennens, D.; Kubota, T.; Le, B.; McDonald, E. F.; Milesi, M.; Nuti, F.; Rados, R.; Scutti, F.; Spiller, L. A.; Tan, K. G.; Taylor, G. N.; Taylor, P. T. E.; Ungaro, F. C.; Urquijo, R.; Volpi, M.; Zanzi, D.] Univ Melbourne, Sch Phys, Melbourne, Vic, Australia.
[Amidei, D.; Chelstowska, M. A.; Cheng, H. C.; Dai, T.; Diehl, E. B.; Edgar, R. C.; Feng, H.; Ferretti, C.; Fleischmann, P.; Guan, L.; Levin, D.; Liu, H.; Lu, N.; Marley, D. E.; Mc Kee, S. P.; McCarn, A.; Neal, H. A.; Qian, J.; Schwarz, T. A.; Searcy, J.; Sekhon, K.; Wu, Y.; Yu, J. M.; Zhang, D.; Zhou, B.; Zhu, J.] Univ Michigan, Dept Phys, Ann Arbor, MI 48109 USA.
[Arabidze, G.; Brock, R.; Chegwidden, A.; Fisher, W. C.; Halladjian, G.; Hauser, R.; Hayden, D.; Huston, J.; Martin, B.; Mondragon, M. C.; Plucinski, P.; Pope, B. G.; Schoenrock, B. D.; Schwienhorst, R.; Willis, C.] Michigan State Univ, Dept Phys & Astron, E Lansing, MI 48824 USA.
[Alimonti, G.; Andreazza, A.; Camplani, A.; Carminati, L.; Cavalli, D.; Citterio, M.; Costa, G.; Fanti, M.; Giugni, D.; Lari, T.; Lazzaroni, M.; Mandelli, L.; Manzoni, S.; Mazza, S. M.; Meroni, C.; Monzani, S.; Perini, L.; Ragusa, F.; Ratti, M. G.; Resconi, S.; Shojaii, S.; Stabile, A.; Tartarelli, G. F.; Troncon, C.; Turra, R.; Perez, M. Villaplana] Ist Nazl Fis Nucl, Sez Milano, Milan, Italy.
[Andreazza, A.; Camplani, A.; Carminati, L.; Fanti, M.; Lazzaroni, M.; Manzoni, S.; Mazza, S. M.; Monzani, S.; Perini, L.; Ragusa, F.; Ratti, M. G.; Shojaii, S.; Turra, R.; Perez, M. Villaplana] Univ Milan, Dipartimento Fis, Milan, Italy.
[Harkusha, S.; Kulchitsky, Y.; Kurochkin, Y. A.; Tsiareshka, P. V.] Natl Acad Sci Belarus, BI Stepanov Phys Inst, Minsk, Byelarus.
[Hrynevich, A.] Natl Sci & Educ Ctr Particle & High Energy Phys, Minsk, Byelarus.
[Arguin, J-F.; Azuelos, G.; Dallaire, F.; Ducu, O. A.; Gagnon, L. G.; Gauthier, L.; Leroy, C.; Mochizuki, K.; Manh, T. Nguyen; Rezvani, R.; Saadi, D. Shoaleh] Univ Montreal, Grp Particle Phys, Montreal, PQ, Canada.
[Akimov, A. V.; Gavrilenko, I. L.; Komar, A. A.; Mashinistov, R.; Mouraviev, S. V.; Nechaeva, P. Yu.; Shmeleva, A.; Snesarev, A. A.; Sulin, V. V.; Tikhomirov, V. O.; Zhukov, K.] Russian Acad Sci, PN Lebedev Phys Inst, Moscow, Russia.
[Artamonov, A.; Gorbounov, P. A.; Khovanskiy, V.; Shatalov, P. B.; Tsukerman, I. I.] ITEP, Moscow, Russia.
[Antonov, A.; Belotskiy, K.; Belyaev, N. L.; Bulekov, O.; Dolgoshein, B. A.; Kantserov, V. A.; Krasnopevtsev, D.; Romaniouk, A.; Shulga, E.; Smirnov, S. Yu.; Smirnov, Y.; Soldatov, E. Yu.; Timoshenko, S.; Vorobev, K.] Natl Res Nucl Univ MEPhI, Moscow, Russia.
[Gladilin, L. K.; Kramarenko, V. A.; Maevskiy, A.; Sivoklokov, S. Yu.; Smirnova, L. N.; Turchikhin, S.] Moscow MV Lomonosov State Univ, DV Skobeltsyn Inst Nucl Phys, Moscow, Russia.
[Adomeit, S.; Bender, M.; Biebel, O.; Bock, C.; Calfayan, P.; Chow, B. K. B.; Duckeck, G.; Hartmann, N. M.; Heinrich, J. J.; Hertenberger, R.; Hoenig, F.; Legger, F.; Lorenz, J.; Losel, P-J; Maier, T.; Mann, A.; Mehlhase, S.; Meineck, C.; Mitrevski, J.; Mueller, R. S. P.; Rauscher, F.; Ruschke, A.; Schachtner, B. M.; Schaile, D.; Unverdorben, C.; Valderanis, C.; Walkerioi, R.; Wittkowski, J.] Ludwig Maximilians Univ Munchen, Fak Phys, Munich, Germany.
[Compostella, G.; Cortiana, G.; Ecker, K. M.; Flowerdew, M. J.; Giuliani, C.; Goblirsch-Kolb, M.; Kiryunin, A. E.; Kortner, O.; Kroha, H.; La Rosa, A.; Macchiolo, A.; Maier, A. A.; Mueller, F.; Oberlack, H.; Salihagic, D.; Schacht, R.; Schmidt-Sommerfeld, K. R.; Schwegler, Ph.; Spettel, F.; von der Schmitt, H.; Wildauer, A.] Werner Heisenberg Inst, Max Planck Inst Phys, Munich, Germany.
[Fusayasu, T.; Shimojima, M.] Nagasaki Inst Appl Sci, Nagasaki, Japan.
[Horii, Y.; Kentaro, K.; Onogi, K.; Tomoto, M.; Wakabayashi, J.; Yamauchi, K.] Nagoya Univ, Grad Sch Sci, Nagoya, Aichi, Japan.
[Horii, Y.; Kentaro, K.; Onogi, K.; Tomoto, M.; Wakabayashi, J.; Yamauchi, K.] Nagoya Univ, Kobayashi Maskawa Inst, Nagoya, Aichi, Japan.
[Aloisio, A.; Alviggi, M. G.; Canale, V.; Carlino, G.; Cirotto, F.; Conventi, F.; de Asmundis, R.; Della Pietra, M.; Doria, A.; Izzo, V.; Merola, L.; Perrella, S.; Rossi, E.; Sanchez, A.; Sekhniaidze, G.] Ist Nazl Fis Nucl, Sez Napoli, Naples, Italy.
[Aloisio, A.; Alviggi, M. G.; Canale, V.; Cirotto, F.; Merola, L.; Perrella, S.; Rossi, E.; Sanchez, A.] Univ Napoli, Dipartimento Fis, Naples, Italy.
[Gorelov, I.; Hoeferkamp, M. R.; Mc Fadden, N. C.; Seidel, S. C.; Taylor, A. C.; Toms, K.] Univ New Mexico, Dept Phys & Astron, Albuquerque, NM 87131 USA.
[Caron, S.; Colasurdo, L.; Croft, V.; De Groot, N.; Filthaut, F.; Galea, C.; Konig, A. C.; Nektarijevic, S.; Strubig, A.] Radboud Univ Nijmegen Nikhef, Inst Math Astrophys & Particle Phys, Nijmegen, Netherlands.
[Aben, R.; Angelozzi, I.; Bedognetti, M.; Beemster, L. J.; Bentvelsen, S.; Berge, D.; Bobbink, G. J.; Bos, K.; Brenner, L.; Bruni, L. S.; Butti, P.; Castelijn, R.; Castelli, A.; Colijn, A. P.; de Jong, P.; Deigaard, I.; Duda, D.; Ferrari, P.; Hartjes, F.; Hessey, N. P.; Igonkina, O.; Kluit, R.; Koffeman, E.; Mahlstedt, J.; Meyer, J.; Oussoren, K. P.; Sabato, G.; Salek, D.; Slawinska, M.; Valencic, N.; Van den Wollenberg, W.; Van der Deij, Rc.; van der Geer, R.; van der Graaf, H.; van Vulpen, I.; Vankov, R.; Verkerke, W.; Vermeulen, C.; Vreeswijk, M.; Weits, H.; Williams, S.] Nikhef Natl Inst Subat Phys, Amsterdam, Netherlands.
[Aben, R.; Angelozzi, I.; Bedognetti, M.; Beemster, L. J.; Bentvelsen, S.; Berge, D.; Bobbink, G. J.; Bos, K.; Brenner, L.; Bruni, L. S.; Butti, P.; Castelijn, R.; Castelli, A.; Colijn, A. P.; de Jong, P.; Deigaard, I.; Duda, D.; Ferrari, P.; Hartjes, F.; Hessey, N. P.; Igonkina, O.; Kluit, R.; Koffeman, E.; Mahlstedt, J.; Meyer, J.; Oussoren, K. P.; Sabato, G.; Salek, D.; Slawinska, M.; Valencic, N.; Van den Wollenberg, W.; Van der Deij, Rc.; van der Geer, R.; van der Graaf, H.; van Vulpen, I.; Vankov, R.; Verkerke, W.; Vermeulen, C.; Vreeswijk, M.; Weits, H.; Williams, S.] Univ Amsterdam, Amsterdam, Netherlands.
[Adelman, J.; Andari, N.; Burghgrave, B.; Chakraborty, D.; Klimek, R.; Saha, R.] Northern Illinois Univ, Dept Phys, De Kalb, IL USA.
[Anisenkov, A. V.; Baldin, E. M.; Bobrovnikov, V. S.; Bogdanchikov, A. G.; Buzykaev, A. R.; Kazanin, V. F.; Kharlamov, A. G.; Korol, A. A.; Maslennikov, A. L.; Maximov, D. A.; Peleganchuk, S. V.; Rezanova, O. L.; Soukharev, A. M.; Talyshev, A. A.; Tikhonov, Yu. A.] RAS, SB, Budker Inst Nucl Phys, Novosibirsk, Russia.
[Becot, C.; Bernius, C.; Cranmer, K.; Haas, A.; Heinrich, L.; Kaplan, B.; Karthik, K.; Konoplich, R.; Mincer, A. I.; Nemethy, R.; Neves, R. M.] NYU, Dept Phys, 4 Washington Pl, New York, NY 10003 USA.
[Beacham, J. B.; Che, S.; Gan, K. K.; Ishmukhametov, R.; Kagan, H.; Kass, R. D.; Looper, K. A.; Shrestha, S.; Tannenwald, B. B.] Ohio State Univ, Columbus, OH 43210 USA.
[Nakano, I.] Okayama Univ, Fac Sci, Okayama, Japan.
[Abbott, B.; Alhroob, M.; Bertsche, D.; De Benedetti, A.; Gutierrez, R.; Hasib, A.; Norberg, S.; Pearson, B.; Rifki, O.; Severini, H.; Strauss, M.] Univ Oklahoma, Homer L Dodge Dept Phys & Astron, Norman, OK 73019 USA.
[Cantero, J.; Haley, J.; Jamin, D. O.; Khanov, A.; Rizatdinova, F.; Sidorov, D.] Oklahoma State Univ, Dept Phys, Stillwater, OK 74078 USA.
[Chytka, L.; Hamal, R.; Hrabovsky, M.; Kvita, J.; Nozka, L.] Palacky Univ, RCPTM, Olomouc, Czech Republic.
[Abreu, R.; Allen, B. W.; Brau, J. E.; Brost, E.; Hopkins, W. H.; Majewski, S.; Potter, C. T.; Radloff, R.; Sinev, N. B.; Strom, D. M.; Torrence, E.; Wanotayaroj, C.; Whalen, K.; Winklmeier, F.] Univ Oregon, Ctr High Energy Phys, Eugene, OR 97403 USA.
[Abeloos, B.; Ayoub, M. K.; Bassalat, A.; Binet, S.; Bourdarios, C.; De Regie, J. B. De Vivie; Delgove, D.; Duflot, L.; Escalier, M.; Fayard, L.; Fournier, D.; Gkougkousis, E. L.; Goudet, C. R.; Grivaz, J. -F.; Hariri, F.; Henrot-Versille, S.; Hrivnac, J.; Iconomidou-Fayard, L.; Kado, M.; Lounis, A.; Maiani, C.; Makovec, N.; Morange, N.; Nellist, C.; Petroff, R.; Poggioli, L.; Puzo, P.; Rousseau, D.; Rybkin, G.; Schaffer, A. C.; Serin, L.; Simion, S.; Tanaka, R.; Zerwas, D.; Zhang, Z.] Univ Paris Saclay, Univ Paris Sud, CNRS, LAL,IN2P3, Orsay, France.
[Endo, M.; Nomachi, M.; Sugaya, Y.; Teoh, J. J.; Yamaguchi, Y.] Osaka Univ, Grad Sch Sci, Osaka, Japan.
[Bugge, M. K.; Cameron, D.; Catmore, J. R.; Feigl, S.; Franconi, L.; Garonne, V.; Gjelsten, B. K.; Gramstad, E.; Morisbak, V.; Nilsen, J. K.; Ould-Saada, F.; Pajchel, K.; Pedersen, M.; Raddum, S.; Read, A. L.; Rohne, O.; Sandaker, H.; Serfon, C.; Stapnes, S.; Strandlie, A.] Univ Oslo, Dept Phys, Oslo, Norway.
[Artoni, G.; Barr, A. J.; Becker, K.; Beresford, L.; Bortoletto, D.; Burr, J. T. P.; Cooper-Sarkar, A. M.; Ortuzar, M. Crispin; Fawcett, W. J.; Frost, J. A.; Gallas, E. J.; Giuli, F.; Gupta, S.; Gwenlan, C.; Hays, C. P.; Henderson, J.; Huffman, T. B.; Issever, C.; Kalderon, C. W.; Nagai, K.; Nickerson, R. B.; Norjoharuddeen, N.; Petrov, M.; Pickering, M. A.; Tseng, J. C-L.; Viehhauser, G. H. A.; Vigani, L.; Weidberg, A. R.; Zhong, J.] Univ Oxford, Dept Phys, Oxford, England.
[Dondero, P.; Farina, E. M.; Ferrari, R.; Fraternali, M.; Gaudio, G.; Introzzi, G.; Lanza, A.; Livan, M.; Negri, A.; Polesello, G.; Rebuzzi, D. M.; Rimoldi, A.; Vercesi, V.] Ist Nazl Fis Nucl, Sez Pavia, Pavia, Italy.
[Dondero, P.; Farina, E. M.; Fraternali, M.; Introzzi, G.; Livan, M.; Negri, A.; Rebuzzi, D. M.; Rimoldi, A.] Univ Pavia, Dipartimento Fis, Pavia, Italy.
[Balunas, W. K.; Brendlinger, K.; Di Clemente, W. K.; Fletcher, R. R. M.; Haney, B.; Heim, S.; Hines, E.; Jackson, B.; Kroll, J.; Lipeles, E.; Miguens, J. Machado; Meyer, C.; Mistry, K. P.; Reichert, J.; Thomson, E.; Vanguri, R.; Williams, H. H.; Yoshihara, K.] Univ Penn, Dept Phys, Philadelphia, PA 19104 USA.
[Basalaev, A.; Ezhilov, A.; Fedin, O. L.; Gratchev, V.; Levchenko, M.; Maleev, V. P.; Naryshkin, I.; Ryabov, Y. F.; Schegelsky, V. A.; Seliverstov, D. M.] BP Konstantinov Petersburg Nucl Phys Inst, Kurchatov Inst, Natl Res Ctr, St Petersburg, Russia.
[Annovi, A.; Bertolucci, F.; Biesuz, N. V.; Cavasinni, V.; Chiarelli, G.; Del Prete, T.; Dell'Orso, M.; Donati, S.; Giannetti, P.; Leone, S.; Roda, C.; Scuri, F.; Sotiropoulou, C. L.; Spalla, M.; Volpi, G.] Ist Nazl Fis Nucl, Sez Pisa, Pisa, Italy.
[Annovi, A.; Bertolucci, F.; Biesuz, N. V.; Cavasinni, V.; Chiarelli, G.; Del Prete, T.; Dell'Orso, M.; Donati, S.; Giannetti, P.; Leone, S.; Roda, C.; Scuri, F.; Sotiropoulou, C. L.; Spalla, M.; Volpi, G.] Univ Pisa, Dipartimento Fis E Fermi, Pisa, Italy.
[Bianchi, R. M.; Boudreau, J.; Escobar, C.; Farina, C.; Hong, T. M.; Mueller, J.; Sapp, K.; Su, J.] Univ Pittsburgh, Dept Phys & Astron, Pittsburgh, PA 15260 USA.
[Aguilar-Saavedra, J. A.; Amor Dos Santos, S. P.; Amorim, A.; Araque, J. P.; Cantrill, R.; Carvalho, J.; Castro, N. F.; Conde Muino, P.; Da Cunha Sargedas De Sousa, M. J.; Fiolhais, M. C. N.; Galhardo, B.; Gomes, A.; Goncalo, R.; Jorge, P. M.; Lopes, L.; Maio, A.; Maneira, J.; Seabra, L. F. Oleiro; Onofre, A.; Palma, A.; Pedro, R.; Santos, H.; Saraiva, J. G.; Silva, J.; Delgado, A. Tavares; Veloso, F.; Wolters, H.] LIP, Lab Instrumentacao & Fis Expt Particulas, Lisbon, Portugal.
[Amorim, A.; Conde Muino, P.; Da Cunha Sargedas De Sousa, M. J.; Gomes, A.; Jorge, P. M.; Miguens, J. Machado; Maio, A.; Maneira, J.; Palma, A.; Pedro, R.; Delgado, A. Tavares] Univ Lisbon, Fac Ciencias, Lisbon, Portugal.
[Amor Dos Santos, S. P.; Carvalho, J.; Fiolhais, M. C. N.; Galhardo, B.; Veloso, F.; Wolters, H.] Univ Coimbra, Dept Phys, Coimbra, Portugal.
[Gomes, A.; Maio, A.; Saraiva, J. G.; Silva, J.] Univ Lisbon, Ctr Fis Nucl, Lisbon, Portugal.
[Onofre, A.] Univ Minho, Dept Fis, Braga, Portugal.
[Aguilar-Saavedra, J. A.] Univ Granada, Dept Fis Teor & Cosmos, Granada, Spain.
[Aguilar-Saavedra, J. A.] Univ Granada, CAFPE, Granada, Spain.
Univ Nova Lisboa, Dept Fis, Fac Ciencias & Tecnol, Caparica, Portugal.
Univ Nova Lisboa, CEFITEC, Fac Ciencias & Tecnol, Caparica, Portugal.
[Chudoba, J.; Havranek, M.; Hejbal, J.; Jakoubek, T.; Kepka, O.; Kupco, A.; Kus, V.; Lokajicek, M.; Lysak, R.; Marcisovsky, M.; Mikestikova, M.; Nemecek, S.; Penc, O.; Sicho, R.; Staroba, R.; Svatos, M.; Tasevsky, M.] Acad Sci Czech Republic, Inst Phys, Prague, Czech Republic.
[Ali, B.; Augsten, K.; Caforio, D.; Gallus, P.; Hubacek, Z.; Myska, M.; Pospisil, S.; Seifert, F.; Simak, V.; Slavicek, T.; Smolek, K.; Solar, M.; Sopczak, A.; Sopko, V.; Suk, M.; Turecek, D.; Vacek, V.; Vlasak, M.; Vokac, R.; Vykyda, Z.; Zeman, M.] Czech Tech Univ, Prague, Czech Republic.
[Balek, P.; Berta, P.; Carli, I.; Davidek, T.; Dolejsi, J.; Dolezal, Z.; Faltova, J.; Kodys, P.; Kosek, T.; Leitner, R.; Reznicek, R.; Scheirich, D.; Slovak, R.; Spousta, M.; Sykora, T.; Tas, R.; Todorova-Nova, S.; Valkar, S.; Vorobel, V.] Charles Univ Prague, Fac Math & Phys, Prague, Czech Republic.
[Borisov, A.; Cheremushkina, E.; Denisov, S. P.; Fakhrutdinov, R. M.; Fenyuk, A. B.; Golubkov, D.; Kamenshchikov, A.; Karyukhin, A. N.; Kozhin, A. S.; Minaenko, A. A.; Myagkov, A. G.; Nikolaenko, V.; Ryzhov, A.; Solodkov, A. A.; Solovyanov, O. V.; Starchenko, E. A.; Vaniachine, A.; Zaitsev, A. M.; Zenin, O.] NRC KI, State Res Ctr Inst High Energy Phys Protvino, Protvino, Russia.
[Adye, T.; Baines, J. T.; Barnett, B. M.; Burke, S.; Dewhurst, A.; Dopke, J.; Emeliyanov, D.; Gallop, B. J.; Gee, C. N. P.; Haywood, S. J.; Kirk, J.; Martin-Haugh, S.; McMahon, S. J.; Middleton, R. P.; Murray, W. J.; Phillips, P. W.; Sankey, D. P. C.; Sawyer, C.; Tyndel, M.; Wickens, F. J.; Wielers, M.; Worm, S. D.] Rutherford Appleton Lab, Particle Phys Dept, Didcot, Oxon, England.
[Anulli, F.; Bagiacchi, P.; Bagnaia, P.; Bauce, M.; Bini, C.; Ciapetti, G.; Corradi, M.; De Pedis, D.; De Salvo, A.; Di Donato, C.; Falciano, S.; Gentile, S.; Giagu, S.; Gustavino, G.; Kuna, M.; Lacava, F.; Luci, C.; Luminari, L.; Messina, A.; Nisati, A.; Pasqualucci, E.; Petrolo, E.; Rescignona, M.; Rosati, S.; Tehrani, F. Safai; Vanadia, M.; Vari, R.; Veneziano, S.; Verducci, M.; Zanello, L.] Ist Nazl Fis Nucl, Sez Roma, Rome, Italy.
[Bagiacchi, P.; Bagnaia, P.; Bauce, M.; Bini, C.; Ciapetti, G.; Corradi, M.; Di Donato, C.; Gentile, S.; Giagu, S.; Gustavino, G.; Kuna, M.; Lacava, F.; Luci, C.; Messina, A.; Vanadia, M.; Verducci, M.; Zanello, L.] Sapienza Univ Roma, Dipartimento Fis, Rome, Italy.
[Aielli, G.; Camarri, P.; Cardarelli, R.; Di Ciaccio, A.; Iuppa, R.; Liberti, B.; Salamona, A.; Santonico, R.] Ist Nazl Fis Nucl, Sez Roma Tor Vergata, Rome, Italy.
[Aielli, G.; Camarri, P.; Di Ciaccio, A.; Iuppa, R.; Salamona, A.; Santonico, R.] Univ Roma Tor Vergata, Dipartimento Fis, Rome, Italy.
[Baroncelli, A.; Biglietti, M.; Ceradini, F.; Di Micco, B.; Farilla, A.; Graziani, E.; Iodice, M.; Orestano, D.; Petrucci, F.; Puddu, D.; Salamanna, G.; Sessa, M.; Stanescu, C.; Taccini, C.] Ist Nazl Fis Nucl, Sez Roma Tre, Rome, Italy.
[Ceradini, F.; Di Micco, B.; Orestano, D.; Petrucci, F.; Puddu, D.; Salamanna, G.; Sessa, M.; Taccini, C.] Univ Roma Tre, Dipartimento Matemat & Fis, Rome, Italy.
[Benchekroun, D.; Chafaq, A.; Hoummada, A.] Univ Hassan 2, Reseau Univ Phys Hautes Energies, Fac Sci Ain Chock, Casablanca, Morocco.
[Ghazlane, H.] Ctr Natl Energie Sci Tech Nucl, Rabat, Morocco.
[El Kacimi, M.; Goujdami, D.; Haddad, N.] Univ Cadi Ayyad, LPHEA Marrakech, Fac Sci Semlalia, Marrakech, Morocco.
[Aaboud, M.; Derkaoui, J. E.; Ouchrif, M.; Tayalati, Y.] Univ Mohamed Premier, Fac Sci, Oujda, Morocco.
[Aaboud, M.; Derkaoui, J. E.; Ouchrif, M.; Tayalati, Y.] LPTPM, Oujda, Morocco.
[El Moursli, R. Cherkaoui; Fassi, F.; Idrissi, Z.] Univ Mohammed 5, Fac Sci, Rabat, Morocco.
[Bachacou, H.; Balli, F.; Bauer, F.; Besson, N.; Blanchard, J. -B.; Boonekamp, M.; Chevalier, L.; Hoffmann, M. Dano; Deliot, F.; Denysiuk, D.; Etienvre, A. I.; Formica, A.; Giraud, P. F.; Da Costa, J. Goncalves Pinto Firmino; Guyot, C.; Hanna, R.; Hassani, S.; Jeanneau, F.; Kivernyk, O.; Kozanecki, W.; Kukla, R.; Lancon, E.; Laporte, J. F.; Le Quilleuc, E. P.; Lesage, A. A. J.; Mansoulie, B.; Meyer, J. -R; Nicolaidou, R.; Ouraou, A.; Rodriguez, L. Pacheco; Perego, M. M.; Peyaud, A.; Royon, C. R.; Saimpert, M.; Schoeffel, L.; Schune, Ph.; Schwemling, Ph.; Schwindling, J.] Commissariat Energie Atom & Energies Alternat, CEA Saclay, Inst Rech Lois Fondamentales Univers, DSM IRFU, Gif Sur Yvette, France.
[AbouZeid, O. S.; Battaglia, M.; Debenedetti, C.; Grillo, A. A.; Hance, M.; Kuhl, A.; Law, A. T.; Litke, A. M.; Lockman, W. S.; Nielsen, J.; Rose, P.; Sadrozinski, H. F-W.; Schier, S.; Schumm, B. A.; Seiden, A.] Univ Calif Santa Cruz, Santa Cruz Inst Particle Phys, Santa Cruz, CA 95064 USA.
[Alpigiani, C.; Blackburn, D.; Goussiou, A. G.; Hsu, S-C.; Johnson, W. J.; Lubatti, H. J.; Marx, M.; Meehan, S.; Rompotis, N.; Rosten, R.; Rothberg, J.; Russell, H. L.; De Bruin, P. H. Sales; Pastor, E. Torro; Watts, G.; Whallon, N. L.] Univ Washington, Dept Phys, Seattle, WA 98195 USA.
[Anastopoulos, C.; Costanzo, D.; Donszelmann, T. Cuhadar; Dawson, I.; Fletcher, G. T.; Hamity, G. N.; Hodgkinson, M. C.; Hodgson, R.; Johansson, P.; Klinger, J. A.; Korolkova, E. V.; Kyriazopoulos, D.; Paredes, B. Lopez; Macdonald, C. M.; Miyagawa, P. S.; Parker, K. A.; Tovey, D. R.; Vickey, T.; Boeriu, O. E. Vickey] Univ Sheffield, Dept Phys & Astron, Sheffield, S Yorkshire, England.
[Hasegawa, Y.; Takeshita, T.] Shinshu Univ, Dept Phys, Nagano, Japan.
[Atlay, N. B.; Buchholz, P.; Campoverde, A.; Czirr, H.; Fleck, I.; Gaur, B.; Ghasemi, S.; Ibragimov, I.; Li, Y.; Rosenthal, O.; Walkowiak, W.; Ziolkowski, M.] Univ Siegen, Fachbereich Phys, Siegen, Germany.
[Buat, Q.; Horton, A. J.; Mori, D.; O'Neil, D. C.; Pachal, K.; Stelzer, B.; Temple, D.; Torres, H.; Van Nieuwkoop, J.; Vetterli, M. C.] Simon Fraser Univ, Dept Phys, Burnaby, BC, Canada.
[Armbruster, A. J.; Barklow, T.; Bartoldus, R.; Bawa, H. S.; Black, J. E.; Gao, Y. S.; Garelli, N.; Grenier, R.; Ilic, N.; Kagan, M.; Kocian, M.; Koi, T.; Malone, C.; Moss, J.; Mount, R.; Nachman, B. P.; Nef, P. D.; Piacquadio, G.; Rubbo, F.; Salnikov, A.; Schwartzman, A.; Skubic, R.; Su, D.; Tompkins, L.; Wittgen, M.; Young, C.; Zeng, Q.] SLAC Natl Accelerator Lab, Stanford, CA USA.
[Astalos, R.; Bartos, P.; Blazek, T.; Dado, T.; Melo, M.; Plazak, L.; Smiesko, J.; Sykora, I.; Tokar, S.; Zenis, T.] Comenius Univ, Fac Math Phys & Informat, Bratislava, Slovakia.
[Bruncko, D.; Kladiva, E.; Strizenec, P.; Urban, J.] Slovak Acad Sci, Inst Expt Phys, Dept Subnucl Phys, Kosice, Slovakia.
[Castaneda-Miranda, E.; Hamilton, A.; Yacoob, S.] Univ Cape Town, Dept Phys, Cape Town, South Africa.
[Connell, S. H.; Govender, N.] Univ Johannesburg, Dept Phys, Johannesburg, South Africa.
[Hsu, C.; Kar, D.; Garcia, B. R. Mellado; Ruan, X.] Univ Witwatersrand, Sch Phys, Johannesburg, South Africa.
[Abulaiti, Y.; Akerstedt, H.; Asman, B.; Bendtz, K.; Bertoli, G.; Bylund, O. Bessidskaia; Bohm, C.; Clement, C.; Cribbs, W. A.; Hellman, S.; Jon-And, K.; Lundberg, O.; Milstead, D. A.; Moa, T.; Molander, S.; Pani, R.; Poettgen, R.; Rossetti, V.; Shaikh, N. W.; Shcherbakova, A.; Silverstein, S. B.; Sjolin, J.; Strandberg, S.; Ughetto, M.; Santurio, E. Valdes; Wallangen, V.] Stockholm Univ, Dept Phys, Stockholm, Sweden.
[Abulaiti, Y.; Akerstedt, H.; Asman, B.; Bendtz, K.; Bertoli, G.; Clement, C.; Cribbs, W. A.; Hellman, S.; Jon-And, K.; Lundberg, O.; Milstead, D. A.; Moa, T.; Molander, S.; Pani, R.; Poettgen, R.; Rossetti, V.; Shaikh, N. W.; Shcherbakova, A.; Sjolin, J.; Strandberg, S.; Ughetto, M.; Santurio, E. Valdes; Wallangen, V.] Oskar Klein Ctr, Stockholm, Sweden.
[Lund-Jensen, B.; Sidebo, P. E.; Strandberg, J.] Royal Inst Technol, Dept Phys, Stockholm, Sweden.
[Balestri, T.; Bee, C. P.; Chen, K.; Hobbs, J.; Huo, R.; Jia, J.; Li, H.; Lindquist, B. E.; McCarthy, R. L.; Montalbano, A.; Morvaj, L.; Radhakrishnan, S. K.; Rijssenbeek, M.; Schamberger, R. D.; Tsybychev, D.; Zaman, A.; Zhou, M.] SUNY Stony Brook, Dept Phys & Astron, Stony Brook, NY 11794 USA.
[Balestri, T.; Bee, C. P.; Chen, K.; Hobbs, J.; Huo, R.; Jia, J.; Li, H.; Lindquist, B. E.; McCarthy, R. L.; Montalbano, A.; Morvaj, L.; Radhakrishnan, S. K.; Rijssenbeek, M.; Schamberger, R. D.; Tsybychev, D.; Zaman, A.; Zhou, M.] SUNY Stony Brook, Dept Chem, Stony Brook, NY 11794 USA.
[Abraham, N. L.; Allbrooke, B. M. M.; Asquith, L.; Cerri, A.; Barajas, C. A. Chavez; De Sanctis, U.; De Santo, A.; Grout, Z. J.; Lerner, G.; Miano, F.; Salvatore, F.; Castillo, I. Santoyo; Shehu, C. Y.; Suruliz, K.; Sutton, M. R.; Vivarelli, I.; Winston, O. J.] Univ Sussex, Dept Phys & Astron, Brighton, E Sussex, England.
[Black, C. W.; Cuthbert, C.; Finelli, K. D.; Jeng, G. -Y.; Limosani, A.; Morley, A. K.; Saavedra, A. F.; Scarcella, M.; Varvell, K. E.; Wang, J.; Yabsley, B.] Univ Sydney, Sch Phys, Sydney, NSW, Australia.
[Hou, S.; Hsu, P. J.; Lee, S. C.; Lin, S. C.; Liu, B.; Liu, D.; Lo Sterzo, F.; Mazini, R.; Shi, L.; Soh, D. A.; Teng, P. K.; Wang, S. M.; Yang, Y.] Acad Sinica, Inst Phys, Taipei, Taiwan.
[Abreu, H.; Gozani, E.; Rozen, Y.; Tarem, S.; van Eldik, N.] Technion Israel Inst Technol, Dept Phys, Haifa, Israel.
[Abramowicz, H.; Alexander, G.; Ashkenazi, A.; Bella, G.; Benary, O.; Benhammou, Y.; Davies, M.; Duarte-Campderros, J.; Etzion, E.; Gershon, A.; Gueta, O.; Oren, Y.; Soffer, A.; Taiblum, N.] Tel Aviv Univ, Raymond & Beverly Sackler Sch Phys & Astron, Tel Aviv, Israel.
[Gkaitatzis, S.; Gkialas, I.; Iliadis, D.; Kimura, N.; Kordas, K.; Kourkoumeli-Charalampidi, A.; Leisos, A.; Papageorgiou, K.; Petridou, C.; Sampsonidis, D.] Aristotle Univ Thessaloniki, Dept Phys, Thessaloniki, Greece.
[Asai, S.; Chen, S.; Dohmae, T.; Enari, Y.; Hanawa, K.; Kanaya, N.; Kataoka, Y.; Kato, C.; Kawamoto, T.; Kazama, S.; Kobayashi, A.; Kobayashi, T.; Komori, Y.; Kozakai, C.; Mashimo, T.; Masubuchi, T.; Minami, Y.; Mori, T.; Morinaga, M.; Nakamura, T.; Ninomiya, Y.; Nobe, T.; Saito, T.; Sakamoto, H.; Sasaki, Y.; Tanaka, J.; Terashi, K.; Ueda, I.; Yamamoto, S.; Yamanaka, T.] Univ Tokyo, Int Ctr Elementary Particle Phys, Tokyo, Japan.
[Asai, S.; Chen, S.; Dohmae, T.; Enari, Y.; Hanawa, K.; Kanaya, N.; Kataoka, Y.; Kato, C.; Kawamoto, T.; Kazama, S.; Kobayashi, A.; Kobayashi, T.; Komori, Y.; Kozakai, C.; Mashimo, T.; Masubuchi, T.; Minami, Y.; Mori, T.; Morinaga, M.; Nakamura, T.; Ninomiya, Y.; Nobe, T.; Saito, T.; Sakamoto, H.; Sasaki, Y.; Tanaka, J.; Terashi, K.; Ueda, I.; Yamamoto, S.; Yamanaka, T.] Univ Tokyo, Dept Phys, Tokyo, Japan.
[Bratzler, U.; Fukunaga, C.] Tokyo Metropolitan Univ, Grad Sch Sci & Technol, Tokyo, Japan.
[Ishitsuka, M.; Jinnouchi, O.; Kobayashi, D.; Kuze, M.; Motohashi, K.; Todome, K.; Yamaguchi, D.] Tokyo Inst Technol, Dept Phys, Tokyo, Japan.
[Batista, S. J.; Chau, C. C.; Cormier, K. J. R.; DeMarco, D. A.; Di Sipio, R.; Diamond, M.; Keoshkerian, H.; Krieger, P.; Liblong, A.; Mc Goldrick, G.; Orr, R. S.; Pascuzzi, V. R.; Polifka, R.; Rudolph, M. S.; Savard, R.; Sinervo, R.; Taenzer, J.; Teuscher, R. J.; Trischuk, W.; Veloce, L. M.; Venturi, N.] Univ Toronto, Dept Phys, Toronto, ON, Canada.
[Canepa, A.; Chekulaev, S. V.; Hod, N.; Jovicevic, J.; Codina, E. Perez; Schneider, B.; Stelzer-Chilton, O.; Tafirout, R.; Trigger, I. M.] TRIUMF, Vancouver, BC, Canada.
[Ramos, J. Manjarres; Palacino, G.; Taylor, W.] York Univ, Dept Phys & Astron, Toronto, ON, Canada.
[Hara, K.; Ito, F.; Kasahara, K.; Kim, S. H.; Kiuchi, K.; Nagata, K.; Okawa, H.; Sato, K.; Ukegawa, F.] Univ Tsukuba, Fac Pure & Appl Sci, Tsukuba, Ibaraki, Japan.
[Hara, K.; Ito, F.; Kasahara, K.; Kim, S. H.; Kiuchi, K.; Nagata, K.; Okawa, H.; Sato, K.; Ukegawa, F.] Univ Tsukuba, Ctr Integrated Res Fundamental Sci & Engn, Tsukuba, Ibaraki, Japan.
[Beauchemin, P. H.; Meoni, E.; Shwa, K.; Son, H.; Wetter, J.] Tufts Univ, Dept Phys & Astron, Medford, MA 02155 USA.
[Casper, D. W.; Corso-Radu, A.; Frate, M.; Guest, D.; Lankford, A. J.; Mete, A. S.; Nelson, A.; Scannicchio, D. A.; Schernau, M.; Shimmin, C. O.; Taffard, A.; Unel, G.; Whiteson, D.] Univ Calif Irvine, Dept Phys & Astron, Irvine, CA 92697 USA.
[Acharya, B. S.; Boldyrev, A. S.; Cobal, M.; Giordani, M. P.; Pinamonti, M.; Quayle, W. B.; Serkin, L.; Shaw, K.; Soualah, R.; Truong, L.] Ist Nazl Fis Nucl, Grp Collegato Udine, Sez Trieste, Udine, Italy.
[Acharya, B. S.; Quayle, W. B.; Serkin, L.; Shaw, K.] Abdus Salaam Int Ctr Theoret Phys, Trieste, Italy.
[Boldyrev, A. S.; Cobal, M.; Giordani, M. P.; Pinamonti, M.; Soualah, R.; Truong, L.] Univ Udine, Dipartimento Chim Fis & Ambiente, Udine, Italy.
[Kuutmann, E. Bergeaas; Brenner, R.; Ekelof, T.; Ellert, M.; Ferrari, A.; Maddocks, H. J.; Ohman, H.; Rangel-Smith, C.] Uppsala Univ, Dept Phys & Astron, Uppsala, Sweden.
[Atkinson, M.; Armadans, R. Caminal; Cavaliere, V.; Chang, P.; Errede, S.; Hooberman, B. H.; Khader, M.; Lie, K.; Liss, T. M.; Liu, L.; Long, J. D.; Outschoorn, V. I. Martinez; Neubauer, M. S.; Pontecorvo, L.; Rybar, M.; Shang, R.; Sickles, A. M.; Vichou, I.; Zeng, J. C.] Univ Illinois, Dept Phys, 1110 W Green St, Urbana, IL 61801 USA.
[Piqueras, D. Alvarez; Barranco Navarro, L.; Cabrera Urban, S.; Castillo Gimenez, V.; Cerda Alberich, L.; Costa, M. J.; Fernandez Martinez, P.; Ferrer, A.; Fiorini, L.; Fuster, J.; Garcia, C.; Navarro, J. E. Garcia; de la Hoz, S. Gonzalez; Jimenez, Y. Hernandez; Higon-Rodriguez, E.; Pena, J. Jimenez; King, M.; Lacasta, C.; Lacuesta, V. R.; Mamuzic, J.; Marti-Garcia, S.; Melini, D.; Mitsou, V. A.; Lopez, S. Pedraza; Rodriguez Rodriguez, D.; Adam, E. Romero; Ros, E.; Salt, J.; Sanchez, J.; Martinez, V. Sanchez; Soldevila, U.; Valero, A.; Ferrer, J. A. Valls; Vos, M.] Univ Valencia, Inst Fis Corpuscular IFIC, Valencia, Spain.
[Piqueras, D. Alvarez; Barranco Navarro, L.; Cabrera Urban, S.; Castillo Gimenez, V.; Cerda Alberich, L.; Costa, M. J.; Fernandez Martinez, P.; Ferrer, A.; Fiorini, L.; Fuster, J.; Garcia, C.; Navarro, J. E. Garcia; de la Hoz, S. Gonzalez; Jimenez, Y. Hernandez; Higon-Rodriguez, E.; Pena, J. Jimenez; King, M.; Lacasta, C.; Lacuesta, V. R.; Mamuzic, J.; Marti-Garcia, S.; Melini, D.; Mitsou, V. A.; Lopez, S. Pedraza; Rodriguez Rodriguez, D.; Adam, E. Romero; Ros, E.; Salt, J.; Sanchez, J.; Martinez, V. Sanchez; Soldevila, U.; Valero, A.; Ferrer, J. A. Valls; Vos, M.] Univ Valencia, Dept Fis Atom Mol & Nucl, Valencia, Spain.
[Piqueras, D. Alvarez; Barranco Navarro, L.; Cabrera Urban, S.; Castillo Gimenez, V.; Cerda Alberich, L.; Costa, M. J.; Fernandez Martinez, P.; Ferrer, A.; Fiorini, L.; Fuster, J.; Garcia, C.; Navarro, J. E. Garcia; de la Hoz, S. Gonzalez; Jimenez, Y. Hernandez; Higon-Rodriguez, E.; Pena, J. Jimenez; King, M.; Lacasta, C.; Lacuesta, V. R.; Mamuzic, J.; Marti-Garcia, S.; Melini, D.; Mitsou, V. A.; Lopez, S. Pedraza; Rodriguez Rodriguez, D.; Adam, E. Romero; Ros, E.; Salt, J.; Sanchez, J.; Martinez, V. Sanchez; Soldevila, U.; Valero, A.; Ferrer, J. A. Valls; Vos, M.] Univ Valencia, Dept Ingn Elect, Valencia, Spain.
[Piqueras, D. Alvarez; Barranco Navarro, L.; Cabrera Urban, S.; Castillo Gimenez, V.; Cerda Alberich, L.; Costa, M. J.; Fernandez Martinez, P.; Ferrer, A.; Fiorini, L.; Fuster, J.; Garcia, C.; Navarro, J. E. Garcia; de la Hoz, S. Gonzalez; Jimenez, Y. Hernandez; Higon-Rodriguez, E.; Pena, J. Jimenez; King, M.; Lacasta, C.; Lacuesta, V. R.; Mamuzic, J.; Marti-Garcia, S.; Melini, D.; Mitsou, V. A.; Lopez, S. Pedraza; Rodriguez Rodriguez, D.; Adam, E. Romero; Ros, E.; Salt, J.; Sanchez, J.; Martinez, V. Sanchez; Soldevila, U.; Valero, A.; Ferrer, J. A. Valls; Vos, M.] Univ Valencia, IMB, CNM, Valencia, Spain.
[Piqueras, D. Alvarez; Barranco Navarro, L.; Cabrera Urban, S.; Castillo Gimenez, V.; Cerda Alberich, L.; Costa, M. J.; Fernandez Martinez, P.; Ferrer, A.; Fiorini, L.; Fuster, J.; Garcia, C.; Navarro, J. E. Garcia; de la Hoz, S. Gonzalez; Jimenez, Y. Hernandez; Higon-Rodriguez, E.; Pena, J. Jimenez; King, M.; Lacasta, C.; Lacuesta, V. R.; Maeda, J.; Mamuzic, J.; Marti-Garcia, S.; Melini, D.; Mitsou, V. A.; Lopez, S. Pedraza; Rodriguez Rodriguez, D.; Adam, E. Romero; Ros, E.; Salt, J.; Sanchez, J.; Martinez, V. Sanchez; Soldevila, U.; Valero, A.; Ferrer, J. A. Valls; Vos, M.] CSIC, Valencia, Spain.
[Danninger, M.; Fedorko, W.; Gay, C.; Gecse, Z.; Gignac, M.; Henkelmann, S.; King, S. B.; Lister, A.; Pelikan, D.; Rettie, S.] Univ British Columbia, Dept Phys, Vancouver, BC, Canada.
[Albert, J.; David, C.; Elliot, A. A.; Fincke-Keeler, M.; Hamano, K.; Hill, E.; Keeler, R.; Kowalewski, R.; Kuwertz, E. S.; Kwan, T.; LeBlanc, M.; Lefebvre, M.; McPherson, R. A.; Pearce, J.; Seuster, R.; Sobie, R.; Trovatelli, M.; Venturi, M.] Univ Victoria, Dept Phys & Astron, Victoria, BC, Canada.
[Beckingham, M.; Ennis, J. S.; Farrington, S. M.; Harrison, P. F.; Jeske, C.; Jones, G.; Martin, T. A.; Murray, W. J.; Pianori, E.; Spangenberg, M.] Univ Warwick, Dept Phys, Coventry, W Midlands, England.
[Iizawa, T.; Mitani, T.; Sakurai, Y.; Yorita, K.] Waseda Univ, Tokyo, Japan.
[Bressler, S.; Citron, Z. H.; Duchovni, E.; Dumancic, M.; Gross, E.; Kohler, M. K.; Lellouch, D.; Levinson, L. J.; Mikenberg, G.; Milov, A.; Pitt, M.; Ravinovich, I.; Roth, I.; Schaarschmidt, J.; Turgeman, D.] Weizmann Inst Sci, Dept Particle Phys, Rehovot, Israel.
[Banerjee, Sw.; Guan, W.; Hard, A. S.; Heng, Y.; Ji, H.; Ju, X.; Kaplan, L. S.; Kashif, L.; Kruse, A.; Ming, Y.; Wang, F.; Wiedenmann, W.; Wu, S. L.; Yang, H.; Zhang, F.; Zobernig, G.] Univ Wisconsin, Dept Phys, 1150 Univ Ave, Madison, WI 53706 USA.
[Kuger, F.; Redelbach, A.; Schreyer, M.; Sidiropoulou, O.; Siragusa, G.; Smakhtin, V.; Strohmer, R.; Trefzger, T.; Weber, S. W.; Zibell, A.] Julius Maximilians Univ, Fak Phys & Astron, Wurzburg, Germany.
[Bannoura, A. A. E.; Boerner, D.; Braun, H. M.; Cornelissen, T.; Ellinghaus, F.; Ernis, G.; Fischer, J.; Flick, T.; Gabizon, O.; Gilles, G.; Hamacher, K.; Harenberg, T.; Hirschbuehl, D.; Kersten, S.; Kuechler, J. T.; Mattig, R.; Neumann, M.; Pataraia, S.; Riegel, C. J.; Sandhoff, M.; Tepel, F.; Vogel, M.; Wagner, W.; Zeitnitz, C.] Berg Univ Wuppertal, Fachgrp Phys, Fak Math & Nat Wissensch, Wuppertal, Germany.
[Baker, O. K.; Noccioli, E. Benhar; Cummings, J.; Demers, S.; Ideal, E.; Lagouri, T.; Leister, A. G.; Loginov, A.; Hernandez, D. Paredes; Thomsen, L. A.; Tipton, R.; Vasquez, J. G.; Wang, X.] Yale Univ, Dept Phys, New Haven, CT USA.
[Hakobyan, H.; Vardanyan, G.] Yerevan Phys Inst, Yerevan, Armenia.
[Rahal, G.] IN2P3, Ctr Calcul, Villeurbanne, France.
[Acharya, B. S.] Kings Coll London, Dept Phys, London, England.
[Ahmadov, F.; Huseynov, N.; Javadov, N.] Azerbaijan Acad Sci, Inst Phys, Baku, Azerbaijan.
[Anisenkov, A. V.; Baldin, E. M.; Bobrovnikov, V. S.; Buzykaev, A. R.; Kazanin, V. F.; Kharlamov, A. G.; Korol, A. A.; Maslennikov, A. L.; Maximov, D. A.; Peleganchuk, S. V.; Rezanova, O. L.; Soukharev, A. M.; Talyshev, A. A.; Tikhonov, Yu. A.] Novosibirsk State Univ, Novosibirsk, Russia.
[Azuelos, G.; Gingrich, D. M.; Oakham, F. G.; Savard, R.; Vetterli, M. C.] TRIUMF, Vancouver, BC, Canada.
[Banerjee, Sw.] Univ Louisville, Dept Phys & Astron, Louisville, KY 40292 USA.
[Bawa, H. S.; Gao, Y. S.] Calif State Univ Fresno, Dept Phys, Fresno, CA 93740 USA.
[Beck, H. P.] Univ Fribourg, Dept Phys, Fribourg, Switzerland.
[Casado, M. P.] Univ Autonoma Barcelona, Dept Fis, Barcelona, Spain.
[Castro, N. F.] Univ Porto, Fac Ciencias, Dept Fis & Astron, Oporto, Portugal.
[Chelkov, G. A.] Tomsk State Univ, Tomsk, Russia.
[Conventi, F.; Della Pietra, M.] Univ Napoli Parthenope, Naples, Italy.
[Corriveau, F.; McPherson, R. A.; Robertson, S. H.; Sobie, R.; Teuscher, R. J.] Inst Particle Phys, Victoria, BC, Canada.
[Ducu, O. A.] Natl Inst Phys & Nucl Engn, Bucharest, Romania.
[Fedin, O. L.] St Petersburg State Polytech Univ, Dept Phys, St Petersburg, Russia.
[Geng, C.; Guo, Y.; Li, B.] Univ Michigan, Dept Phys, Ann Arbor, MI 48109 USA.
[Govender, N.] Ctr High Performance Comp, CSIR Campus, Cape Town, South Africa.
[Greenwood, Z. D.; Sawyer, L.] Louisiana Tech Univ, Ruston, LA 71270 USA.
[Grinstein, S.; Rozas, A. Juste; Martinez, M.] ICREA, Barcelona, Spain.
[Hanagaki, K.] Osaka Univ, Grad Sch Sci, Osaka, Japan.
[Hsu, P. J.] Natl Tsing Hua Univ, Hsinchu, Taiwan.
[Igonkina, O.] Radboud Univ Nijmegen Nikhef, Inst Math Astrophys & Particle Phys, Nijmegen, Netherlands.
[Ilchenko, Y.; Onyisi, P. U. E.] Univ Texas Austin, Dept Phys, Austin, TX 78712 USA.
[Jejelava, J.] Ilia State Univ, Inst Theoret Phys, Tbilisi, Rep of Georgia.
[Jenni, R.] CERN, Geneva, Switzerland.
[Khubua, J.] Georgian Tech Univ, Tbilisi, Rep of Georgia.
[Kono, T.; Nagai, R.] Ochanomizu Univ, Ochadai Acad Prod, Tokyo, Japan.
[Konoplich, R.] Manhattan Coll, New York, NY USA.
[Leisos, A.] Hellen Open Univ, Patras, Greece.
[Lin, S. C.] Acad Sinica, Inst Phys, Acad Sinica Grid Comp, Taipei, Taiwan.
[Liu, B.] Shandong Univ, Sch Phys, Jinan, Shandong, Peoples R China.
[Myagkov, A. G.; Nikolaenko, V.; Zaitsev, A. M.] Moscow Inst Phys & Technol, Dolgoprudnyi, Russia.
[Nessi, M.] Univ Geneva, Sect Phys, Geneva, Switzerland.
[Pasztor, G.] Eotvos Lorand Univ, Budapest, Hungary.
[Pinamonti, M.] Int Sch Adv Studies SISSA, Trieste, Italy.
[Nessi, M.] Univ South Carolina, Dept Phys & Astron, Columbia, SC USA.
[Shi, L.] Sun Yat Sen Univ, Sch Phys & Engn, Guangzhou, Guangdong, Peoples R China.
[Shiyakova, M.] Bulgarian Acad Sci, INRNE, Sofia, Bulgaria.
[Smirnova, L. N.; Turchikhin, S.] Moscow MV Lomonosov State Univ, Fac Phys, Moscow, Russia.
[Song, H. Y.; Zhang, G.] Acad Sinica, Inst Phys, Taipei, Taiwan.
[Tikhomirov, V. O.] Natl Res Nucl Univ MEPhI, Moscow, Russia.
[Tompkins, L.] Stanford Univ, Dept Phys, Stanford, CA 94305 USA.
[Toth, J.; Vest, A.] Wigner Res Ctr Phys, Inst Particle & Nucl Phys, Budapest, Hungary.
Flensburg Univ Appl Sci, Flensburg, Germany.
[Yusuff, I.] Univ Malaya, Dept Phys, Kuala Lumpur, Malaysia.
[Zhang, R.] Aix Marseille Univ, CPPM, Marseille, France.
[Zhang, R.] CNRS, IN2P3, Marseille, France.
PKU CHEP, Beijing, Peoples R China.
[Kuday, S.] Istanbul Aydin Univ, Istanbul, Turkey.
[Sultansoy, S.] TOBB Univ Econ & Technol, Div Phys, Ankara, Turkey.
[Barnovska, Z.; Berger, N.; Delmastro, M.; Di Ciaccio, L.; Elles, S.; Grevtsov, K.; Guillemin, T.; Hryn'ova, T.; Jezequel, S.; Koletsou, I.; Lafaye, R.; Leveque, J.; Mastrandrea, R.; Sauvage, G.; Sauvan, E.; Simard, O.; Smart, B. H.; Todorov, T.; Wingerter-Seez, I.; Yatsenko, E.] Univ Savoie Mt Blanc, Annecy Le Vieux, France.
[Beddall, A.; Bingul, A.] Gaziantep Univ, Dept Engn Phys, Gaziantep, Turkey.
[Cetin, S. A.] Istanbul Bilgi Univ, Fac Engn & Nat Sci, Istanbul, Turkey.
[Beddall, A. J.] Bahcesehir Univ, Fac Engn & Nat Sci, Istanbul, Turkey.
[Cerqueira, A. S.; Manhaes de Andrade Filho, L.; Peralva, B. S.] Univ Fed Juiz de Fora, Elect Circuits Dept, Juiz de Fora, Brazil.
[do Vale, M. A. B.] Fed Univ Sao Joao del Rei UFSJ, Sao Joao Del Rei, Brazil.
[Donadelli, M.; Navarro, J. L. La Rosa; Leite, M. A. L.] Univ Sao Paulo, Inst Fis, Sao Paulo, Brazil.
[Popeneciu, G. A.] Natl Inst Res & Dev Isotop & Mol Technol, Dept Phys, Cluj Napoca, Romania.
Univ Politehn Bucuresti, Bucharest, Romania.
[Gravila, P. M.] West Univ Timisoara, Timisoara, Romania.
[Gao, J.; Geng, C.; Guo, Y.; Han, L.; Hu, Q.; Jiang, Y.; Li, B.; Liu, J. B.; Liu, M.; Liu, Y. L.; Liu, Y.; Peng, H.; Song, H. Y.; Wang, W.; Zhang, G.; Zhang, R.; Zhao, Z.; Zhu, Y.] Univ Sci & Technol China, Dept Modern Phys, Hefei, Anhui, Peoples R China.
[Chen, S.; Wang, C.; Zhang, H.] Nanjing Univ, Dept Phys, Nanjing, Jiangsu, Peoples R China.
[Du, Y.; Feng, C.; Ma, L. L.; Ma, Y.; Wang, C.; Zaidan, R.; Zhang, X.; Zhao, Y.; Zhu, C. G.] Shandong Univ, Sch Phys, Jinan, Shandong, Peoples R China.
[Bret, M. Cano; Guo, J.; Li, L.; Yang, H.] Shanghai Jiao Tong Univ, Dept Phys & Astron, Shanghai Key Lab Particle Phys & Cosmol, Shanghai, Peoples R China.
[Chen, X.; Zhou, N.] Tsinghua Univ, Dept Phys, Beijing 100084, Peoples R China.
[Palka, M.; Richter-Was, E.] Jagiellonian Univ, Marian Smoluchowski Inst Phys, Krakow, Poland.
[Kretz, M.; Kugel, A.] Heidelberg Univ, ZITI Inst Tech Informat, Mannheim, Germany.
RP Aaboud, M (reprint author), Univ Mohamed Premier, Fac Sci, Oujda, Morocco.; Aaboud, M (reprint author), LPTPM, Oujda, Morocco.
RI Kuday, Sinan/C-8528-2014; Soldatov, Evgeny/E-3990-2017; Doyle,
Anthony/C-5889-2009; Mitsou, Vasiliki/D-1967-2009; Solodkov,
Alexander/B-8623-2017; Camarri, Paolo/M-7979-2015; Carvalho,
Joao/M-4060-2013; Prokoshin, Fedor/E-2795-2012; Livan,
Michele/D-7531-2012; Guo, Jun/O-5202-2015; Gladilin, Leonid/B-5226-2011;
Villa, Mauro/C-9883-2009; Peleganchuk, Sergey/J-6722-2014; messina,
andrea/C-2753-2013; Yang, Haijun/O-1055-2015; White, Ryan/E-2979-2015;
Li, Liang/O-1107-2015; Monzani, Simone/D-6328-2017; Warburton,
Andreas/N-8028-2013; Tikhomirov, Vladimir/M-6194-2015
OI Belanger-Champagne, Camille/0000-0003-2368-2617; Belyaev,
Nikita/0000-0002-1131-7121; Lazzaroni, Massimo/0000-0002-4094-1273;
Kuday, Sinan/0000-0002-0116-5494; Soldatov, Evgeny/0000-0003-0694-3272;
Doyle, Anthony/0000-0001-6322-6195; Mitsou,
Vasiliki/0000-0002-1533-8886; Solodkov, Alexander/0000-0002-2737-8674;
Camarri, Paolo/0000-0002-5732-5645; Carvalho, Joao/0000-0002-3015-7821;
Prokoshin, Fedor/0000-0001-6389-5399; Prokofiev,
Kirill/0000-0002-2177-6401; Veneziano, Stefano/0000-0002-2598-2659;
Lacasta, Carlos/0000-0002-2623-6252; Livan, Michele/0000-0002-5877-0062;
Guo, Jun/0000-0001-8125-9433; Gladilin, Leonid/0000-0001-9422-8636;
Villa, Mauro/0000-0002-9181-8048; Peleganchuk,
Sergey/0000-0003-0907-7592; White, Ryan/0000-0003-3589-5900; Li,
Liang/0000-0001-6411-6107; Monzani, Simone/0000-0002-0479-2207;
Warburton, Andreas/0000-0002-2298-7315; Tikhomirov,
Vladimir/0000-0002-9634-0581
FU ANPCyT, Argentina; YerPhI, Armenia; ARC, Australia; BMWFW, Austria; FWF,
Austria; ANAS, Azerbaijan; SSTC, Belarus; CNPq, Brazil; FAPESP, Brazil;
NSERC, Canada; NRC, Canada; CFI, Canada; CERN; CONICYT, Chile; CAS,
China; MOST, China; NSFC, China; COLCIENCIAS, Colombia; MSMT CR, Czech
Republic; MPO CR, Czech Republic; VSC CR, Czech Republic; DNRF, Denmark;
DNSRC, Denmark; IN2P3-CNRS, France; CEA-DSM/IRFU, France; GNSF, Georgia;
BMBF, Germany; HGF, Germany; MPG, Germany; GSRT, Greece; RGC, China;
Hong Kong SAR, China; ISF, Israel; I-CORE, Israel; Benoziyo Center,
Israel; INFN, Italy; MEXT, Japan; JSPS, Japan; CNRST, Morocco; FOM,
Netherlands; NWO, Netherlands; RCN, Norway; MNiSW, Poland; NCN, Poland;
FCT, Portugal; MNE/IFA, Romania; MES of Russia, Russian Federation; NRC
KI, Russian Federation; JINR; MESTD, Serbia; MSSR, Slovakia; ARRS,
Slovenia; MIZS, Slovenia; DST/NRF, South Africa; MINECO, Spain; SRC,
Sweden; Knut and Alice Wallenberg Foundation, Sweden; SERI, Switzerland;
SNSF, Switzerland; Canton of Bern, Switzerland; Canton of Geneva,
Switzerland; MOST, Taiwan; TAEK, Turkey; STFC, United Kingdom; DOE,
United States; NSF, United States; BCKDF, Canada; Canada Council,
Canada; CANARIE, Canada; CRC, Canada; Compute Canada, Canada; FQRNT,
Canada; Ontario Innovation Trust, Canada; EPLANET, European Union; ERC,
European Union; FP7, European Union; Horizon 2020, European Union; Marie
Sklodowska-Curie Actions, European Union; Investissements d'Avenir Labex
and Idex, France; ANR, France; Region Auvergne, France; Fondation
Partager le Savoir, France; DFG, Germany; AvH Foundation, Germany;
Herakleitos; Thales; Aristeia programmes; EU-ESF; Greek NSRF; BSF,
Israel; GIF, Israel; Minerva, Israel; BRF, Norway; Generalitat de
Cataluna, Spain; Generalitat Valenciana, Spain; Royal Society, United
Kingdom; Leverhulme Trust, United Kingdom
FX We acknowledge the support of ANPCyT, Argentina; YerPhI, Armenia; ARC,
Australia; BMWFW and FWF, Austria; ANAS, Azerbaijan; SSTC, Belarus; CNPq
and FAPESP, Brazil; NSERC, NRC and CFI, Canada; CERN; CONICYT, Chile;
CAS, MOST and NSFC, China; COLCIENCIAS, Colombia; MSMT CR, MPO CR and
VSC CR, Czech Republic; DNRF and DNSRC, Denmark; IN2P3-CNRS,
CEA-DSM/IRFU, France; GNSF, Georgia; BMBF, HGF, and MPG, Germany; GSRT,
Greece; RGC, Hong Kong SAR, China; ISF, I-CORE and Benoziyo Center,
Israel; INFN, Italy; MEXT and JSPS, Japan; CNRST, Morocco; FOM and NWO,
Netherlands; RCN, Norway; MNiSW and NCN, Poland; FCT, Portugal; MNE/IFA,
Romania; MES of Russia and NRC KI, Russian Federation; JINR; MESTD,
Serbia; MSSR, Slovakia; ARRS and MIZS, Slovenia; DST/NRF, South Africa;
MINECO, Spain; SRC and Knut and Alice Wallenberg Foundation, Sweden;
SERI, SNSF and Cantons of Bern and Geneva, Switzerland; MOST, Taiwan;
TAEK, Turkey; STFC, United Kingdom; DOE and NSF, United States. In
addition, individual groups and members have received support from
BCKDF, the Canada Council, CANARIE, CRC, Compute Canada, FQRNT, and the
Ontario Innovation Trust, Canada; EPLANET, ERC, FP7, Horizon 2020 and
Marie Sklodowska-Curie Actions, European Union; Investissements d'Avenir
Labex and Idex, ANR, Region Auvergne and Fondation Partager le Savoir,
France; DFG and AvH Foundation, Germany; Herakleitos, Thales and
Aristeia programmes co-financed by EU-ESF and the Greek NSRF; BSF, GIF
and Minerva, Israel; BRF, Norway; Generalitat de Catalunya, Generalitat
Valenciana, Spain; the Royal Society and Leverhulme Trust, United
Kingdom.
NR 58
TC 3
Z9 3
U1 24
U2 24
PU ELSEVIER SCIENCE BV
PI AMSTERDAM
PA PO BOX 211, 1000 AE AMSTERDAM, NETHERLANDS
SN 0370-2693
EI 1873-2445
J9 PHYS LETT B
JI Phys. Lett. B
PD OCT 10
PY 2016
VL 761
BP 372
EP 392
DI 10.1016/j.physletb.2016.08.055
PG 21
WC Astronomy & Astrophysics; Physics, Nuclear; Physics, Particles & Fields
SC Astronomy & Astrophysics; Physics
GA DX6CI
UT WOS:000384469900053
ER
PT J
AU Alexandrou, K
Masurkar, A
Edrees, H
Wishart, JF
Hao, YF
Petrone, N
Hone, J
Kymissis, I
AF Alexandrou, Konstantinos
Masurkar, Amrita
Edrees, Hassan
Wishart, James F.
Hao, Yufeng
Petrone, Nicholas
Hone, James
Kymissis, Ioannis
TI Improving the radiation hardness of graphene field effect transistors
SO APPLIED PHYSICS LETTERS
LA English
DT Article
ID RAMAN-SPECTROSCOPY; DEVICES; IRRADIATION; ELECTRONICS; SCATTERING;
DEFECTS
AB Ionizing radiation poses a significant challenge to the operation and reliability of conventional silicon-based devices. Here, we report the effects of gamma radiation on graphene field-effect transistors (GFETs), along with a method to mitigate those effects by developing a radiation-hardened version of our back-gated GFETs. We demonstrate that activated atmospheric oxygen from the gamma ray interaction with air damages the semiconductor device, and damage to the substrate contributes additional threshold voltage instability. Our radiation-hardened devices, which have protection against these two effects, exhibit minimal performance degradation, improved stability, and significantly reduced hysteresis after prolonged gamma radiation exposure. We believe this work provides an insight into graphene's interactions with ionizing radiation that could enable future graphene-based electronic devices to be used for space, military, and other radiationsensitive applications. Published by AIP Publishing.
C1 [Alexandrou, Konstantinos; Masurkar, Amrita; Edrees, Hassan; Kymissis, Ioannis] Columbia Univ, Dept Elect Engn, New York, NY 10027 USA.
[Wishart, James F.] Brookhaven Natl Lab, Div Chem, Upton, NY 11973 USA.
[Hao, Yufeng; Petrone, Nicholas; Hone, James] Columbia Univ, Dept Mech Engn, New York, NY 10027 USA.
RP Alexandrou, K (reprint author), Columbia Univ, Dept Elect Engn, New York, NY 10027 USA.
EM kka2114@columbia.edu
RI Wishart, James/L-6303-2013; Kymissis, Ioannis/A-5994-2010;
OI Wishart, James/0000-0002-0488-7636; Kymissis,
Ioannis/0000-0001-7417-1759; Petrone, Nicholas/0000-0003-1995-4077
FU NSF MRSEC program through Columbia in the Center for Precision Assembly
of Superstratic and Superatomic Solids [DMR-1420634]; Defense Threat
Reduction Agency (DTRA) [HDTRA1-11-0022]; US-DOE Office of Science,
Division of Chemical Sciences, Geosciences and Biosciences
[DE-AC02-98CH10886, DE-SC0012704]
FX This material is based upon the work supported by the NSF MRSEC program
through Columbia in the Center for Precision Assembly of Superstratic
and Superatomic Solids (DMR-1420634) and the Defense Threat Reduction
Agency (DTRA) under HDTRA1-11-0022. The work at BNL and use of the
60Co source of the BNL Accelerator Center for Energy Research
were supported by the US-DOE Office of Science, Division of Chemical
Sciences, Geosciences and Biosciences under Contract Nos.
DE-AC02-98CH10886 and DE-SC0012704.
NR 36
TC 1
Z9 1
U1 28
U2 28
PU AMER INST PHYSICS
PI MELVILLE
PA 1305 WALT WHITMAN RD, STE 300, MELVILLE, NY 11747-4501 USA
SN 0003-6951
EI 1077-3118
J9 APPL PHYS LETT
JI Appl. Phys. Lett.
PD OCT 10
PY 2016
VL 109
IS 15
AR 153108
DI 10.1063/1.4963782
PG 5
WC Physics, Applied
SC Physics
GA EA3VI
UT WOS:000386534800047
ER
PT J
AU Cao, YW
Park, SY
Liu, XR
Choudhury, D
Middey, S
Meyers, D
Kareev, M
Shafer, P
Arenholz, E
Chakhalian, J
AF Cao, Yanwei
Park, Se Young
Liu, Xiaoran
Choudhury, D.
Middey, S.
Meyers, D.
Kareev, M.
Shafer, P.
Arenholz, E.
Chakhalian, J.
TI Orbital configuration in CaTiO3 films on NdGaO3
SO APPLIED PHYSICS LETTERS
LA English
DT Article
ID ROOM-TEMPERATURE FERROELECTRICITY; 2-DIMENSIONAL ELECTRON GASES;
AUGMENTED-WAVE METHOD; OXIDE INTERFACES; LAALO3/SRTIO3 INTERFACE;
THIN-FILMS; BATIO3; SRTIO3; SUPERCONDUCTIVITY; FERROMAGNETISM
AB Despite its use as a constituent layer for realization of a polar metal and interfacial conductivity, the microscopic study of electronic structure of CaTiO3 is still very limited. Here, we epitaxially stabilized CaTiO3 films on NdGaO3 (110) substrates in a layer-by-layer way by pulsed laser deposition. The structural and electronic properties of the films were characterized by reflection-high-energy-electron-diffraction, X-ray diffraction, and element-specific resonant X-ray absorption spectroscopy. To reveal the orbital polarization and the crystal field splitting of the titanium 3d state, X-ray linear dichroism was carried out on CaTiO3 films, demonstrating the orbital configuration of d(xz)/d(yz)3 target. J.C. and Y.C. acknowledge the support by the
Gordon and Betty Moore Foundation EPiQS Initiative through Grant No.
GBMF4534. X.L. was supported by the Department of Energy Grant No.
DE-SC0012375 for his synchrotron work. S.M., and M.K. were supported by
the DOD-ARO under Grant No. 0402-17291. The Advanced Light Source is
supported by the Director, Office of Science, Office of Basic Energy
Sciences, of the U.S. Department of Energy under Contract No.
DE-AC02-05CH11231. The first-principles calculations were performed on
the Rutgers University Parallel Computer (RUPC) cluster and supported by
the Office of Naval Research Grant No. N00014-14-1-0613.
NR 49
TC 0
Z9 0
U1 10
U2 10
PU AMER INST PHYSICS
PI MELVILLE
PA 1305 WALT WHITMAN RD, STE 300, MELVILLE, NY 11747-4501 USA
SN 0003-6951
EI 1077-3118
J9 APPL PHYS LETT
JI Appl. Phys. Lett.
PD OCT 10
PY 2016
VL 109
IS 15
AR 152905
DI 10.1063/1.4964828
PG 5
WC Physics, Applied
SC Physics
GA EA3VI
UT WOS:000386534800039
ER
PT J
AU Li, BZ
Chopdekar, RV
N'Diaye, AT
Mehta, A
Byers, JP
Browning, ND
Arenholz, E
Takamura, Y
AF Li, Binzhi
Chopdekar, Rajesh V.
N'Diaye, Alpha T.
Mehta, Apurva
Byers, J. Paige
Browning, Nigel D.
Arenholz, Elke
Takamura, Yayoi
TI Tuning interfacial exchange interactions via electronic reconstruction
in transition-metal oxide heterostructures
SO APPLIED PHYSICS LETTERS
LA English
DT Article
ID X-RAY-ABSORPTION; SUPERLATTICES; MAGNETS; BIAS; SPECTROSCOPY; FILMS
AB The impact of interfacial electronic reconstruction on the magnetic characteristics of La0.7Sr0.3CoO3 (LSCO)/La0.7Sr0.3MnO3 (LSMO) heterostructures was investigated as a function of layer thickness using a combination of soft x-ray magnetic spectroscopy and bulk magnetometry. We found that the magnetic properties of the LSCO layers are impacted by two competing electronic interactions occurring at the LSCO/substrate and LSMO/LSCO interfaces. For thin LSCO layers (<5 nm), the heterostructures exist in a highly coupled state where the chemically distinct layers behave as a single magnetic compound with magnetically active Co2+ ions. As the LSCO thickness increases, a high coercivity LSCO layer develops which biases a low coercivity layer, which is composed not only of the LSMO layer but also an interfacial LSCO layer. These results suggest an intriguing route to tune the magnetic properties of transition metal oxide heterostructures through careful control of the interface structure. Published by AIP Publishing.
C1 [Li, Binzhi; Chopdekar, Rajesh V.; Byers, J. Paige; Takamura, Yayoi] Univ Calif Davis, Dept Mat Sci & Engn, One Shields Ave, Davis, CA 95616 USA.
[N'Diaye, Alpha T.; Arenholz, Elke] Lawrence Berkeley Natl Lab, Adv Light Source, 1 Cyclotron Rd, Berkeley, CA 94720 USA.
[Mehta, Apurva] SLAC Natl Accelerator Lab, Stanford Synchrotron Radiat Lightsource, Menlo Pk, CA 94025 USA.
[Browning, Nigel D.] Pacific Northwest Natl Lab, Phys & Computat Sci Directorate, Richland, WA 99354 USA.
RP Takamura, Y (reprint author), Univ Calif Davis, Dept Mat Sci & Engn, One Shields Ave, Davis, CA 95616 USA.
EM ytakamura@ucdavis.edu
OI Chopdekar, Rajesh/0000-0001-6727-6501; Takamura,
Yayoi/0000-0002-7946-9279
FU Semiconductor Research Corporation [2309.001]; Office of Science, Office
of Basic Energy Sciences of the U.S. Department of Energy (DOE)
[DE-AC02-05CH11231]; U.S. DOE, Office of Science, Office of Basic Energy
Sciences [DE-AC02-76SF00515]; U.S. DOE [DE-AC05-76RL01830]; U.S. DOE,
Office of Biological and Environmental Research; PNNL
FX This work was supported by the Semiconductor Research Corporation under
Task No. 2309.001. The ALS is supported by the Director, Office of
Science, Office of Basic Energy Sciences, of the U.S. Department of
Energy (DOE) under Contract No. DE-AC02-05CH11231. Use of the SSRL, SLAC
National Accelerator Laboratory, was supported by the U.S. DOE, Office
of Science, Office of Basic Energy Sciences, under Contract No.
DE-AC02-76SF00515. Some of the research described in this paper is part
of the Chemical Imaging Initiative; it was conducted under the
Laboratory Directed Research and Development Program at Pacific
Northwest National Laboratory (PNNL), a multiprogram national laboratory
operated by Battelle for the U.S. DOE under Contract DE-AC05-76RL01830.
A portion of the research was performed using the Environmental
Molecular Sciences Laboratory, a national scientific user facility
sponsored by the U.S. DOE, Office of Biological and Environmental
Research and located at PNNL.
NR 31
TC 0
Z9 0
U1 15
U2 15
PU AMER INST PHYSICS
PI MELVILLE
PA 1305 WALT WHITMAN RD, STE 300, MELVILLE, NY 11747-4501 USA
SN 0003-6951
EI 1077-3118
J9 APPL PHYS LETT
JI Appl. Phys. Lett.
PD OCT 10
PY 2016
VL 109
IS 15
AR 152401
DI 10.1063/1.4964407
PG 5
WC Physics, Applied
SC Physics
GA EA3VI
UT WOS:000386534800028
ER
PT J
AU Wang, X
Rahmani, H
Zhou, J
Gorfien, M
Plaskus, JM
Li, D
Voss, R
Nelson, CA
Lei, KW
Wolcott, A
Zhu, XY
Li, JJ
Cao, JM
AF Wang, Xuan
Rahmani, Hamidreza
Zhou, Jun
Gorfien, Matthew
Plaskus, Joshua Mendez
Li, Dong
Voss, Ryan
Nelson, Cory A.
Lei, Kin Wai
Wolcott, Abraham
Zhu, Xiaoyang
Li, Junjie
Cao, Jianming
TI Ultrafast lattice dynamics in lead selenide quantum dot induced by laser
excitation
SO APPLIED PHYSICS LETTERS
LA English
DT Article
ID COHERENT ACOUSTIC PHONONS; CARRIER-MULTIPLICATION; PBSE NANOCRYSTALS;
MICROCRYSTALLITES; PHOTOGENERATION; DIFFRACTION; GENERATION; MECHANISMS;
EFFICIENCY
AB We directly monitored the lattice dynamics in PbSe quantum dots (QD) induced by laser excitation using ultrafast electron diffraction. The energy relaxation between the carriers and the lattice took place within 10 ps, showing no evidence of any significant phonon bottleneck effect. Meanwhile, the lattice dilation exhibited some unusual features that could not be explained by the available mechanisms of photon-induced acoustic vibrations in semiconductors alone. The heat transport between the QDs and the substrate deviates significantly from Fourier's Law, which opens questions about the heat transfer under nonequilibrium conditions in nanoscale materials. Published by AIP Publishing.
C1 [Wang, Xuan] Chinese Acad Sci, Inst Phys, POB 603, Beijing 100190, Peoples R China.
[Rahmani, Hamidreza; Zhou, Jun; Gorfien, Matthew; Plaskus, Joshua Mendez; Li, Dong; Voss, Ryan; Cao, Jianming] Florida State Univ, Dept Phys, Tallahassee, FL 32310 USA.
[Rahmani, Hamidreza; Zhou, Jun; Gorfien, Matthew; Plaskus, Joshua Mendez; Li, Dong; Voss, Ryan; Cao, Jianming] Florida State Univ, Natl High Magnet Field Lab, Tallahassee, FL 32310 USA.
[Nelson, Cory A.; Lei, Kin Wai; Wolcott, Abraham; Zhu, Xiaoyang] Columbia Univ, Dept Chem, New York, NY 10027 USA.
[Li, Junjie] Brookhaven Natl Lab, Condensed Matter Phys & Mat Sci Dept, Upton, NY 11973 USA.
RP Wang, X (reprint author), Chinese Acad Sci, Inst Phys, POB 603, Beijing 100190, Peoples R China.; Cao, JM (reprint author), Florida State Univ, Dept Phys, Tallahassee, FL 32310 USA.; Wang, X; Cao, JM (reprint author), Florida State Univ, Natl High Magnet Field Lab, Tallahassee, FL 32310 USA.
EM xw@iphy.ac.cn; jcao@magnet.fsu.edu
FU Internal Research Program of Institute of Physics Chinese Academy of
Sciences; National Science Foundation of USA [1207252]; National Science
Foundation [DMR-1157490]; State of Florida
FX This work is supported by the Internal Research Program of Institute of
Physics Chinese Academy of Sciences, the National Science Foundation of
USA (Grant No. 1207252), National Science Foundation Cooperative
Agreement No. DMR-1157490 and the State of Florida.
NR 38
TC 0
Z9 0
U1 23
U2 23
PU AMER INST PHYSICS
PI MELVILLE
PA 1305 WALT WHITMAN RD, STE 300, MELVILLE, NY 11747-4501 USA
SN 0003-6951
EI 1077-3118
J9 APPL PHYS LETT
JI Appl. Phys. Lett.
PD OCT 10
PY 2016
VL 109
IS 15
AR 153105
DI 10.1063/1.4964269
PG 5
WC Physics, Applied
SC Physics
GA EA3VI
UT WOS:000386534800044
ER
PT J
AU Melnicki, MR
Leverenz, RL
Sutter, M
Lopez-Igual, R
Wilson, A
Pawlowski, EG
Perreau, F
Kirilovsky, D
Kerfeld, CA
AF Melnicki, Matthew R.
Leverenz, Ryan L.
Sutter, Markus
Lopez-Igual, Rocio
Wilson, Adjele
Pawlowski, Emily G.
Perreau, Francois
Kirilovsky, Diana
Kerfeld, Cheryl A.
TI Structure, Diversity, and Evolution of a New Family of Soluble
Carotenoid-Binding Proteins in Cyanobacteria
SO MOLECULAR PLANT
LA English
DT Article
DE carotenoids; cyanobacteria; phylogenomics; protein structure;
photoprotection; molecular evolution
ID MULTIPLE SEQUENCE ALIGNMENT; SYNECHOCYSTIS PCC 6803; SP ATCC 51142;
NOSTOC-PUNCTIFORME; SHOTGUN PROTEOMICS; CRYSTAL-STRUCTURE; STRAIN;
PHOTOPROTECTION; LIGHT; GENE
AB Using a phylogenomic approach, we have identified and subclassified a new family of carotenoid-binding proteins. These proteins have sequence homology to the N-terminal domain (NTD) of the Orange Carotenoid Protein (OCP), and are referred to as Helical Carotenoid Proteins (HCPs). These proteins comprise at least nine distinct clades and are found in diverse organisms, frequently as multiple paralogs representing the distinct clades. These seem to be out-paralogs maintained from ancient duplications associated with subfunctionalization. All of the HCPs share conservation of the residues for carotenoid binding, and we confirm that carotenoid binding is a fundamental property of HCPs. We solved two crystal structures of the Nostoc sp. PCC 7120 HCP1 protein, each binding a different carotenoid, suggesting that the proteins flexibly bind a range of carotenoids. Based on a comprehensive phylogenetic analysis, we propose that one of the HCP subtypes is likely the evolutionary ancestor of the NTD of the OCP, which arose following a domain fusion event. However, we predict that the majority of HCPs have functions distinct from the NTD of the OCP. Our results demonstrate that the HCPs are a new family of functionally diverse carotenoid-binding proteins found among ecophysiologically diverse cyanobacteria.
C1 [Melnicki, Matthew R.; Kerfeld, Cheryl A.] Univ Calif Berkeley, Dept Plant & Microbial Biol, Berkeley, CA 94720 USA.
[Melnicki, Matthew R.; Sutter, Markus; Kerfeld, Cheryl A.] Lawrence Berkeley Natl Lab, Phys Biosci Div, Berkeley, CA 94720 USA.
[Leverenz, Ryan L.; Sutter, Markus; Pawlowski, Emily G.; Kerfeld, Cheryl A.] Michigan State Univ, Dept Biochem & Mol Biol, MSU DOE Plant Res Lab, E Lansing, MI 48824 USA.
[Lopez-Igual, Rocio; Wilson, Adjele; Kirilovsky, Diana] Univ Paris Saclay, Univ Paris 11, CNRS, I2BC,CEA, F-91198 Gif Sur Yvette, France.
[Lopez-Igual, Rocio; Wilson, Adjele; Kirilovsky, Diana] CEA, Inst Biol & Technol Saclay IBiTec S, F-91191 Gif Sur Yvette, France.
[Perreau, Francois] INRA, Inst Jean Pierre Bourgin, UMR 1318, ERL CNRS 3559,Saclay Plant Sci,RD10, F-78026 Versailles, France.
[Lopez-Igual, Rocio] CNRS, UMR 3525, Unite Plast Genome Bacterien, Dept Genomes & Genet,Inst Pasteur, F-75015 Paris, France.
RP Kerfeld, CA (reprint author), Univ Calif Berkeley, Dept Plant & Microbial Biol, Berkeley, CA 94720 USA.; Kerfeld, CA (reprint author), Lawrence Berkeley Natl Lab, Phys Biosci Div, Berkeley, CA 94720 USA.; Kerfeld, CA (reprint author), Michigan State Univ, Dept Biochem & Mol Biol, MSU DOE Plant Res Lab, E Lansing, MI 48824 USA.
EM ckerfeld@lbl.gov
OI Lopez-Igual, Rocio/0000-0002-2369-1583
FU National Science Foundation [IOS 1557324]; Office of Science of the U.S.
Department of Energy [DE-FG02-91ER20021]; Agence Nationale de la
Recherche (ANR, project CYANOPROTECT); Centre National de la Recherche
Scientifique (CNRS); Commissariat a l'Energie Atomique
FX The work in the Kerfeld Laboratory was supported by the National Science
Foundation (IOS 1557324) and by the Office of Science of the U.S.
Department of Energy DE-FG02-91ER20021. The research in D.K.'s
laboratory was supported by grants from the Agence Nationale de la
Recherche (ANR, project CYANOPROTECT), the Centre National de la
Recherche Scientifique (CNRS) and the Commissariat a l'Energie Atomique.
NR 68
TC 1
Z9 1
U1 18
U2 18
PU CELL PRESS
PI CAMBRIDGE
PA 600 TECHNOLOGY SQUARE, 5TH FLOOR, CAMBRIDGE, MA 02139 USA
SN 1674-2052
EI 1752-9867
J9 MOL PLANT
JI Mol. Plant.
PD OCT 10
PY 2016
VL 9
IS 10
BP 1379
EP 1394
DI 10.1016/j.molp.2016.06.009
PG 16
WC Biochemistry & Molecular Biology; Plant Sciences
SC Biochemistry & Molecular Biology; Plant Sciences
GA EA4MG
UT WOS:000386586200003
PM 27392608
ER
PT J
AU Xiang, CX
Weber, AZ
Ardo, S
Berger, A
Chen, YK
Coridan, R
Fountaine, KT
Haussener, S
Hu, S
Liu, R
Lewis, NS
Modestino, MA
Shaner, MM
Singh, MR
Stevens, JC
Sun, K
Walczak, K
AF Xiang, Chengxiang
Weber, Adam Z.
Ardo, Shane
Berger, Alan
Chen, YiKai
Coridan, Robert
Fountaine, Katherine T.
Haussener, Sophia
Hu, Shu
Liu, Rui
Lewis, Nathan S.
Modestino, Miguel A.
Shaner, Matthew M.
Singh, Meenesh R.
Stevens, John C.
Sun, Ke
Walczak, Karl
TI Modeling, Simulation, and Implementation of Solar-Driven Water-Splitting
Devices
SO ANGEWANDTE CHEMIE-INTERNATIONAL EDITION
LA English
DT Review
DE device architecture; hydrogen; modeling; photoelectrochemistry;
solar-driven water splitting
ID WIRELESS PHOTOELECTROCHEMICAL CELLS; MICROWIRE-ARRAY PHOTOELECTRODES;
NAFION THIN-FILMS; HYDROGEN-PRODUCTION; VISIBLE-LIGHT;
ENERGY-CONVERSION; PHOTOCATALYTIC ACTIVITY; TRANSPORT-PROPERTIES;
EXCHANGE MEMBRANES; CURRENT STATE
AB An integrated cell for the solar-driven splitting of water consists of multiple functional components and couples various photoelectrochemical (PEC) processes at different length and time scales. The overall solar-to-hydrogen (STH) conversion efficiency of such a system depends on the performance and materials properties of the individual components as well as on the component integration, overall device architecture, and system operating conditions. This Review focuses on the modeling- and simulation-guided development and implementation of solar-driven water-splitting prototypes from a holistic viewpoint that explores the various interplays between the components. The underlying physics and interactions at the cell level is are reviewed and discussed, followed by an overview of the use of the cell model to provide target properties of materials and guide the design of a range of traditional and unique device architectures.
C1 [Xiang, Chengxiang; Chen, YiKai; Hu, Shu; Liu, Rui; Lewis, Nathan S.; Shaner, Matthew M.; Sun, Ke] CALTECH, Joint Ctr Artificial Photosynth, Pasadena, CA 91125 USA.
[Weber, Adam Z.; Singh, Meenesh R.; Stevens, John C.; Walczak, Karl] Lawrence Berkeley Natl Lab, Joint Ctr Artificial Photosynth, Berkeley, CA 94720 USA.
[Ardo, Shane] Univ Calif Irvine, Dept Chem, Irvine, CA 92717 USA.
[Ardo, Shane] Univ Calif Irvine, Dept Chem Engn & Mat Sci, Irvine, CA 92717 USA.
[Berger, Alan] Air Prod & Chem Inc, Allentown, PA USA.
[Coridan, Robert] Univ Arkansas, Dept Chem & Biochem, Fayetteville, AR 72701 USA.
[Fountaine, Katherine T.] Northrop Grumman Aerosp Syst, Nanophoton & Plasmon Lab, Redondo Beach, CA USA.
[Haussener, Sophia] Ecole Polytech Fed Lausanne, Lab Renewable Energy Sci & Engn, Lausanne, Switzerland.
[Lewis, Nathan S.; Shaner, Matthew M.; Sun, Ke] CALTECH, Div Chem & Chem Engn, Noyes Lab 210, Pasadena, CA 91125 USA.
[Modestino, Miguel A.] Ecole Polytech Fed Lausanne, Sch Engn, Lausanne, Switzerland.
[Hu, Shu] Yale Univ, Dept Chem & Environm Engn, New Haven, CT 06520 USA.
[Singh, Meenesh R.] Univ Illinois, Dept Chem Engn, Chicago, IL 60680 USA.
RP Xiang, CX (reprint author), CALTECH, Joint Ctr Artificial Photosynth, Pasadena, CA 91125 USA.; Weber, AZ (reprint author), Lawrence Berkeley Natl Lab, Joint Ctr Artificial Photosynth, Berkeley, CA 94720 USA.
EM cxx@caltech.edu; azweber@lbl.gov
RI Sun, Ke /L-4709-2013;
OI Sun, Ke /0000-0001-8209-364X; Weber, Adam/0000-0002-7749-1624; Singh,
Meenesh/0000-0002-3638-8866; Fountaine, Katherine/0000-0002-0414-8227
FU Office of Science of the U.S. Department of Energy [DE-SC0004993]; U.S.
Department of Energy [DE-EE0006963]
FX We would like to thank the community of researchers whose work is
reflected in this Review, especially those past and present at JCAP.
This material is based upon work performed at the Joint Center for
Artificial Photosynthesis (JCAP), a DOE Energy Innovation Hub, supported
through the Office of Science of the U.S. Department of Energy under
Award Number DE-SC0004993. S.A. acknowledges support from the U.S.
Department of Energy under Award No. DE-EE0006963.
NR 147
TC 5
Z9 5
U1 113
U2 113
PU WILEY-V C H VERLAG GMBH
PI WEINHEIM
PA POSTFACH 101161, 69451 WEINHEIM, GERMANY
SN 1433-7851
EI 1521-3773
J9 ANGEW CHEM INT EDIT
JI Angew. Chem.-Int. Edit.
PD OCT 10
PY 2016
VL 55
IS 42
BP 12974
EP 12988
DI 10.1002/anie.201510463
PG 15
WC Chemistry, Multidisciplinary
SC Chemistry
GA DZ4AN
UT WOS:000385799200003
PM 27460923
ER
PT J
AU Latshaw, AM
Chance, WM
Morrison, G
zur Loye, KD
Wilkins, BO
Smith, MD
Whitfield, PS
Kirkham, MJ
Stoian, SA
zur Loye, HC
AF Latshaw, Allison M.
Chance, W. Michael
Morrison, Gregory
zur Loye, Karl D.
Wilkins, Branford O.
Smith, Mark D.
Whitfield, Pamela S.
Kirkham, Melanie J.
Stoian, Sebastian A.
zur Loye, Hans-Conrad
TI Synthesis of a Ferrolite: A Zeolitic All-Iron Framework
SO ANGEWANDTE CHEMIE-INTERNATIONAL EDITION
LA English
DT Article
DE crystal growth; Mossbauer spectroscopy; neutron diffraction; sodalite
structure; zeolites
ID CRYSTAL-GROWTH; MOSSBAUER
AB Crystals of the first sodalite-type zeolite containing an all-iron framework, a ferrolite, Ba-8(Fe12O24)Na-y(OH)(6)center dot xH(2)O, were synthesized using the hydroflux method in nearly quantitative yield. Ba-8(Fe12O24)Na-y(OH)(6)center dot xH(2)O crystallizes in the cubic space group Pm (3) over barm with a = 10.0476-(1) angstrom. Slightly distorted FeO4 tetrahedra are linked to form Fe4O4 and Fe6O6 rings, which in turn yield channels and internal cavities that are characteristic of the sodalite structure. Barium, sodium, and hydroxide ions and water molecules are found in the channels and provide charge balance. Magnetic measurements indicate that the ferrolite exhibits magnetic order up to at least 700 K, with the field-cooled and zero-field-cooled curves diverging. Analysis of the Fe-57 Mossbauer spectra revealed two spectral components that have equal spectral areas, indicating the presence of two subsets of iron centers in the structure. Dehydrated versions of the ferrolite were also prepared by heating the sample.
C1 [Latshaw, Allison M.; Chance, W. Michael; Morrison, Gregory; zur Loye, Karl D.; Wilkins, Branford O.; Smith, Mark D.; zur Loye, Hans-Conrad] Univ South Carolina, Chem & Biochem, Columbia, SC 29208 USA.
[Whitfield, Pamela S.; Kirkham, Melanie J.] Oak Ridge Natl Lab, Oak Ridge, TN 37831 USA.
[Stoian, Sebastian A.] Florida State Univ, Natl High Magnet Field Lab, Tallahassee, FL 32310 USA.
RP zur Loye, HC (reprint author), Univ South Carolina, Chem & Biochem, Columbia, SC 29208 USA.
EM zurloye@mailbox.sc.edu
RI Whitfield, Pamela/P-1885-2015;
OI Whitfield, Pamela/0000-0002-6569-1143; zur Loye,
Hans-Conrad/0000-0001-7351-9098
FU National Science Foundation [DMR-1301757]; U.S. Department of Energy,
Office of Science, Office of Basic Energy Sciences [DE-AC02-06CH11357];
NSF [DMR-1157490]; UCGP project [5064]
FX Financial support for this work was provided by the National Science
Foundation (DMR-1301757) and is gratefully acknowledged. A portion of
this research used resources at the Spallation Neutron Source, a DOE
Office of Science User Facility operated by Oak Ridge National
Laboratory. Use of the Advanced Photon Source at Argonne National
Laboratory was supported by the U.S. Department of Energy, Office of
Science, Office of Basic Energy Sciences (DE-AC02-06CH11357). Part of
this work was performed at the National High Magnetic Field Laboratory
(NHMFL), which is supported by the NSF (DMR-1157490) and the State of
Florida. S.A.S. is an NHMFL Jack E. Crow postdoctoral fellow. The
Mossbauer instrument was funded by the UCGP project 5064 (AO). P.S.W.
thanks Dr. Ovidiu Garlea (SNS, ORNL) for discussions regarding the
magnetic structure determination.
NR 24
TC 0
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U1 21
U2 21
PU WILEY-V C H VERLAG GMBH
PI WEINHEIM
PA POSTFACH 101161, 69451 WEINHEIM, GERMANY
SN 1433-7851
EI 1521-3773
J9 ANGEW CHEM INT EDIT
JI Angew. Chem.-Int. Edit.
PD OCT 10
PY 2016
VL 55
IS 42
BP 13195
EP 13199
DI 10.1002/anie.201607800
PG 5
WC Chemistry, Multidisciplinary
SC Chemistry
GA DZ4AN
UT WOS:000385799200047
PM 27652577
ER
PT J
AU Abe, K
Haga, K
Hayato, Y
Ikeda, M
Iyogi, K
Kameda, J
Kishimoto, Y
Miura, M
Moriyama, S
Nakahata, M
Nakajima, T
Nakano, Y
Nakayama, S
Orii, A
Sekiya, H
Shiozawa, M
Takeda, A
Tanaka, H
Tasaka, S
Tomura, T
Akutsu, R
Kajita, T
Kaneyuki, K
Nishimura, Y
Richard, E
Okumura, K
Labarga, L
Fernandez, P
Blaszczyk, FDM
Gustafson, J
Kachulis, C
Kearns, E
Raaf, JL
Stone, JL
Sulak, LR
Berkman, S
Nantais, CM
Tobayama, S
Goldhaber, M
Kropp, WR
Mine, S
Weatherly, P
Smy, MB
Sobel, HW
Takhistov, V
Ganezer, KS
Hartfiel, BL
Hill, J
Hong, N
Kim, JY
Lim, IT
Park, RG
Himmel, A
Li, Z
O'Sullivan, E
Scholberg, K
Walter, CW
Ishizuka, T
Nakamura, T
Jang, JS
Choi, K
Learned, JG
Matsuno, S
Smith, SN
Friend, M
Hasegawa, T
Ishida, T
Ishii, T
Kobayashi, T
Nakadaira, T
Nakamura, K
Oyama, Y
Sakashita, K
Sekiguchi, T
Tsukamoto, T
Suzuki, AT
Takeuchi, Y
Yano, T
Cao, SV
Hiraki, T
Hirota, S
Huang, K
Jiang, M
Minamino, A
Nakaya, T
Patel, ND
Wendell, RA
Suzuki, K
Fukuda, Y
Itow, Y
Suzuki, T
Mijakowski, P
Frankiewicz, K
Hignight, J
Imber, J
Jung, CK
Li, X
Palomino, JL
Santucci, G
Wilking, MJ
Yanagisawa, C
Fukuda, D
Ishino, H
Kayano, T
Kibayashi, A
Koshio, Y
Mori, T
Sakuda, M
Xu, C
Kuno, Y
Tacik, R
Kim, SB
Okazawa, H
Choi, Y
Nishijima, K
Koshiba, M
Totsuka, Y
Suda, Y
Yokoyama, M
Bronner, C
Calland, RG
Hartz, M
Martens, K
Marti, L
Suzuki, Y
Vagins, MR
Martin, JF
Tanaka, HA
Konaka, A
Chen, S
Wan, L
Zhang, Y
Wilkes, RJ
AF Abe, K.
Haga, K.
Hayato, Y.
Ikeda, M.
Iyogi, K.
Kameda, J.
Kishimoto, Y.
Miura, M.
Moriyama, S.
Nakahata, M.
Nakajima, T.
Nakano, Y.
Nakayama, S.
Orii, A.
Sekiya, H.
Shiozawa, M.
Takeda, A.
Tanaka, H.
Tasaka, S.
Tomura, T.
Akutsu, R.
Kajita, T.
Kaneyuki, K.
Nishimura, Y.
Richard, E.
Okumura, K.
Labarga, L.
Fernandez, P.
Blaszczyk, F. D. M.
Gustafson, J.
Kachulis, C.
Kearns, E.
Raaf, J. L.
Stone, J. L.
Sulak, L. R.
Berkman, S.
Nantais, C. M.
Tobayama, S.
Goldhaber, M.
Kropp, W. R.
Mine, S.
Weatherly, P.
Smy, M. B.
Sobel, H. W.
Takhistov, V.
Ganezer, K. S.
Hartfiel, B. L.
Hill, J.
Hong, N.
Kim, J. Y.
Lim, I. T.
Park, R. G.
Himmel, A.
Li, Z.
O'Sullivan, E.
Scholberg, K.
Walter, C. W.
Ishizuka, T.
Nakamura, T.
Jang, J. S.
Choi, K.
Learned, J. G.
Matsuno, S.
Smith, S. N.
Friend, M.
Hasegawa, T.
Ishida, T.
Ishii, T.
Kobayashi, T.
Nakadaira, T.
Nakamura, K.
Oyama, Y.
Sakashita, K.
Sekiguchi, T.
Tsukamoto, T.
Suzuki, A. T.
Takeuchi, Y.
Yano, T.
Cao, S. V.
Hiraki, T.
Hirota, S.
Huang, K.
Jiang, M.
Minamino, A.
Nakaya, T.
Patel, N. D.
Wendell, R. A.
Suzuki, K.
Fukuda, Y.
Itow, Y.
Suzuki, T.
Mijakowski, P.
Frankiewicz, K.
Hignight, J.
Imber, J.
Jung, C. K.
Li, X.
Palomino, J. L.
Santucci, G.
Wilking, M. J.
Yanagisawa, C.
Fukuda, D.
Ishino, H.
Kayano, T.
Kibayashi, A.
Koshio, Y.
Mori, T.
Sakuda, M.
Xu, C.
Kuno, Y.
Tacik, R.
Kim, S. B.
Okazawa, H.
Choi, Y.
Nishijima, K.
Koshiba, M.
Totsuka, Y.
Suda, Y.
Yokoyama, M.
Bronner, C.
Calland, R. G.
Hartz, M.
Martens, K.
Marti, Ll.
Suzuki, Y.
Vagins, M. R.
Martin, J. F.
Tanaka, H. A.
Konaka, A.
Chen, S.
Wan, L.
Zhang, Y.
Wilkes, R. J.
CA Super-Kamiokande Collaboration
TI SEARCH FOR NEUTRINOS IN SUPER-KAMIOKANDE ASSOCIATED WITH
GRAVITATIONAL-WAVE EVENTS GW150914 AND GW151226
SO ASTROPHYSICAL JOURNAL LETTERS
LA English
DT Article
DE astroparticle physics; gravitational waves; neutrinos
ID BURSTS
AB We report the results from a search in Super-Kamiokande for neutrino signals coincident with the first detected gravitational-wave events, GW150914 and GW151226, as well as LVT151012, using a neutrino energy range from 3.5 MeV to 100. PeV. We searched for coincident neutrino events within a time window of. +/- 500 s around the gravitational-wave detection time. Four neutrino candidates are found for GW150914, and no candidates are found for GW151226. The remaining neutrino candidates are consistent with the expected background events. We calculated the 90% confidence level upper limits on the combined neutrino fluence for both gravitational-wave events, which depends on event energy and topologies. Considering the upward-going muon data set (1.6 GeV-100 PeV), the neutrino fluence limit for each gravitational-wave event is 14-37 (19-50) cm(-2) for muon neutrinos (muon antineutrinos), depending on the zenith angle of the event. In the other data sets, the combined fluence limits for both gravitational-wave events range from 2.4 x 10(4) to 7.0 x 10(9) cm(-2).
C1 [Abe, K.; Haga, K.; Hayato, Y.; Ikeda, M.; Iyogi, K.; Kameda, J.; Kishimoto, Y.; Miura, M.; Moriyama, S.; Nakahata, M.; Nakajima, T.; Nakano, Y.; Nakayama, S.; Orii, A.; Sekiya, H.; Shiozawa, M.; Takeda, A.; Tanaka, H.; Tasaka, S.; Tomura, T.] Univ Tokyo, Inst Cosm Ray Res, Kamioka Observ, Kamioka, Gifu 5061205, Japan.
[Akutsu, R.; Kajita, T.; Kaneyuki, K.; Nishimura, Y.; Richard, E.; Okumura, K.] Univ Tokyo, Res Ctr Cosm Neutrinos, Inst Cosm Ray Res, Kashiwa, Chiba 2778582, Japan.
[Labarga, L.; Fernandez, P.] Univ Autonoma Madrid, Dept Theoret Phys, E-28049 Madrid, Spain.
[Blaszczyk, F. D. M.; Gustafson, J.; Kachulis, C.; Kearns, E.; Raaf, J. L.; Stone, J. L.; Sulak, L. R.] Boston Univ, Dept Phys, Boston, MA 02215 USA.
[Berkman, S.; Nantais, C. M.; Tobayama, S.] Univ British Columbia, Dept Phys & Astron, Vancouver, BC V6T 1Z4, Canada.
[Goldhaber, M.] Brookhaven Natl Lab, Dept Phys, Upton, NY 11973 USA.
[Kropp, W. R.; Mine, S.; Weatherly, P.; Smy, M. B.; Sobel, H. W.; Takhistov, V.; Vagins, M. R.] Univ Calif Irvine, Dept Phys & Astron, Irvine, CA 92697 USA.
[Ganezer, K. S.; Hartfiel, B. L.; Hill, J.] Calif State Univ Dominguez Hills, Dept Phys, Carson, CA 90747 USA.
[Hong, N.; Kim, J. Y.; Lim, I. T.; Park, R. G.] Chonnam Natl Univ, Dept Phys, Kwangju 500757, South Korea.
[Himmel, A.; Li, Z.; O'Sullivan, E.; Scholberg, K.; Walter, C. W.] Duke Univ, Dept Phys, Durham, NC 27708 USA.
[Ishizuka, T.] Fukuoka Inst Technol, Jr Coll, Fukuoka, Fukuoka 8110295, Japan.
[Nakamura, T.] Gifu Univ, Dept Phys, Gifu, Gifu 5011193, Japan.
[Jang, J. S.] Gwangju Inst Sci & Technol, GIST Coll, Gwangju 500712, South Korea.
[Choi, K.; Learned, J. G.; Matsuno, S.; Smith, S. N.] Univ Hawaii, Dept Phys & Astron, Honolulu, HI 96822 USA.
[Friend, M.; Hasegawa, T.; Ishida, T.; Ishii, T.; Kobayashi, T.; Nakamura, K.; Oyama, Y.; Sakashita, K.; Sekiguchi, T.; Tsukamoto, T.] High Energy Accelerator Res Org, KEK, Tsukuba, Ibaraki 3050801, Japan.
[Suzuki, A. T.; Takeuchi, Y.; Yano, T.] Kobe Univ, Dept Phys, Kobe, Hyogo 6578501, Japan.
[Cao, S. V.; Hiraki, T.; Hirota, S.; Huang, K.; Jiang, M.; Minamino, A.; Nakaya, T.; Patel, N. D.; Wendell, R. A.; Suzuki, K.] Kyoto Univ, Dept Phys, Kyoto, Kyoto 6068502, Japan.
[Fukuda, Y.] Miyagi Univ Educ, Dept Phys, Sendai, Miyagi 9800845, Japan.
[Itow, Y.; Suzuki, T.] Nagoya Univ, Inst Space Earth Environm Res, Nagoya, Aichi 4648602, Japan.
[Itow, Y.] Nagoya Univ, Kobayashi Maskawa Inst Origin Particles & Univers, Nagoya, Aichi 4648602, Japan.
[Mijakowski, P.; Frankiewicz, K.] Natl Ctr Nucl Res, PL-00681 Warsaw, Poland.
[Hignight, J.; Imber, J.; Jung, C. K.; Li, X.; Palomino, J. L.; Santucci, G.; Wilking, M. J.; Yanagisawa, C.] SUNY Stony Brook, Dept Phys & Astron, Stony Brook, NY 11794 USA.
[Fukuda, D.; Ishino, H.; Kayano, T.; Kibayashi, A.; Koshio, Y.; Mori, T.; Sakuda, M.; Xu, C.] Okayama Univ, Dept Phys, Okayama, Okayama 7008530, Japan.
[Kuno, Y.] Osaka Univ, Dept Phys, Toyonaka, Osaka 5600043, Japan.
[Tacik, R.] Univ Regina, Dept Phys, 3737 Wascana Pkwy, Regina, SK S4S OA2, Canada.
[Kim, S. B.] Seoul Natl Univ, Dept Phys, Seoul 151742, South Korea.
[Okazawa, H.] Shizuoka Univ Welf, Dept Informat Social Welf, Yaizu, Shizuoka 4258611, Japan.
[Choi, Y.] Sungkyunkwan Univ, Dept Phys, Suwon 440746, South Korea.
[Nishijima, K.] Tokai Univ, Dept Phys, Hiratsuka, Kanagawa 2591292, Japan.
[Koshiba, M.; Totsuka, Y.] Univ Tokyo, Bunkyo Ku, Tokyo 1130033, Japan.
[Suda, Y.; Yokoyama, M.] Univ Tokyo, Dept Phys, Bunkyo Ku, Tokyo 1130033, Japan.
[Abe, K.; Hayato, Y.; Kameda, J.; Kishimoto, Y.; Miura, M.; Moriyama, S.; Nakahata, M.; Nakayama, S.; Sekiya, H.; Shiozawa, M.; Takeda, A.; Tomura, T.; Kajita, T.; Kaneyuki, K.; Okumura, K.; Kearns, E.; Stone, J. L.; Smy, M. B.; Sobel, H. W.; Scholberg, K.; Walter, C. W.; Nakamura, K.; Takeuchi, Y.; Nakaya, T.; Wendell, R. A.; Koshio, Y.; Yokoyama, M.; Bronner, C.; Calland, R. G.; Hartz, M.; Martens, K.; Marti, Ll.; Suzuki, Y.; Vagins, M. R.] Univ Tokyo, Inst Adv Study, Kavli Inst Phys & Math Universe WPI, Kashiwa, Chiba 2778583, Japan.
[Martin, J. F.; Tanaka, H. A.] Univ Toronto, Dept Phys, 60 St George St, Toronto, ON M5S 1A7, Canada.
[Tacik, R.; Konaka, A.] TRIUMF, 4004 Wesbrook Mall, Vancouver, BC V6T 2A3, Canada.
[Chen, S.; Wan, L.; Zhang, Y.] Tsinghua Univ, Dept Engn Phys, Beijing 100084, Peoples R China.
[Wilkes, R. J.] Univ Washington, Dept Phys, Seattle, WA 98195 USA.
[Yanagisawa, C.] CUNY, BMCC, Dept Sci, New York, NY 10021 USA.
RI Nakano, Yuuki/S-2684-2016; Koshio, Yusuke/C-2847-2015
OI Koshio, Yusuke/0000-0003-0437-8505
FU Japanese Ministry of Education, Culture, Sports, Science and Technology;
U.S. Department of Energy; U.S. National Science Foundation; Korean
Research Foundation (BK21); National Research Foundation of Korea
[NRF-20110024009]; European Union (H2020) [RISE-GA641540-SKPLUS]; Japan
Society for the Promotion of Science; National Natural Science
Foundation of China [11235006]; Scinet and Westgrid consortia of Compute
Canada; Korean Research Foundation (KNRC)
FX We gratefully acknowledge the cooperation of the Kamioka Mining and
Smelting Company. The Super-Kamiokande experiment has been built and
operated from funding by the Japanese Ministry of Education, Culture,
Sports, Science and Technology, the U.S. Department of Energy, and the
U.S. National Science Foundation. Some of us have been supported by
funds from the Korean Research Foundation (BK21 and KNRC), the National
Research Foundation of Korea (NRF-20110024009), the European Union
(H2020 RISE-GA641540-SKPLUS), the Japan Society for the Promotion of
Science, the National Natural Science Foundation of China under grant
No. 11235006, and the Scinet and Westgrid consortia of Compute Canada.
NR 22
TC 1
Z9 1
U1 5
U2 5
PU IOP PUBLISHING LTD
PI BRISTOL
PA TEMPLE CIRCUS, TEMPLE WAY, BRISTOL BS1 6BE, ENGLAND
SN 2041-8205
EI 2041-8213
J9 ASTROPHYS J LETT
JI Astrophys. J. Lett.
PD OCT 10
PY 2016
VL 830
IS 1
AR L11
DI 10.3847/2041-8205/830/1/L11
PG 6
WC Astronomy & Astrophysics
SC Astronomy & Astrophysics
GA DZ6AD
UT WOS:000385943000004
ER
PT J
AU Dunlop, JA
Apanaskevich, DA
Lehmann, J
Hoffmann, R
Fusseis, F
Ehlke, M
Zachow, S
Xiao, XH
AF Dunlop, Jason A.
Apanaskevich, Dmitry A.
Lehmann, Jens
Hoffmann, Rene
Fusseis, Florian
Ehlke, Moritz
Zachow, Stefan
Xiao, Xianghui
TI Microtomography of the Baltic amber tick Ixodes succineus reveals
affinities with the modern Asian disease vector Ixodes ovatus
SO BMC EVOLUTIONARY BIOLOGY
LA English
DT Article
DE Arachnida; Parasitiformes; Ixodida; Parasite; Vector; Eocene; Baltic
amber
ID CRETACEOUS BURMESE AMBER; ANAPLASMA-PHAGOCYTOPHILUM; PHYLOGENETIC
ANALYSIS; BORNE ENCEPHALITIS; HARD TICKS; ACARI; IXODIDAE; EVOLUTION;
PARASITIFORMES; SEQUENCES
AB Background: Fossil ticks are extremely rare and Ixodes succineus Weidner, 1964 from Eocene (ca. 44-49 Ma) Baltic amber is one of the oldest examples of a living hard tick genus (Ixodida: Ixodidae). Previous work suggested it was most closely related to the modern and widespread European sheep tick Ixodes ricinus (Linneaus, 1758).
Results: Restudy using phase contrast synchrotron x-ray tomography yielded images of exceptional quality. These confirm the fossil's referral to Ixodes Latreille, 1795, but the characters resolved here suggest instead affinities with the Asian subgenus Partipalpiger Hoogstraal et al., 1973 and its single living (and medically significant) species Ixodes ovatus Neumann, 1899. We redescribe the amber fossil here as Ixodes (Partipalpiger) succineus.
Conclusions: Our data suggest that Ixodes ricinus is unlikely to be directly derived from Weidner's amber species, but instead reveals that the Partipalpiger lineage was originally more widely distributed across the northern hemisphere. The closeness of Ixodes (P.) succineus to a living vector of a wide range of pathogens offers the potential to correlate its spatial and temporal position (northern Europe, nearly 50 million years ago) with the estimated origination dates of various tick-borne diseases.
C1 [Dunlop, Jason A.] Leibniz Inst Res Evolut & Biodivers, Museum Nat Kunde, Invalidenstr 43, D-10115 Berlin, Germany.
[Apanaskevich, Dmitry A.] Georgia Southern Univ, James H Oliver Jr Inst Coastal Plain Sci, US Natl Tick Collect, Statesboro, GA 30460 USA.
[Lehmann, Jens] Univ Bremen, Fac Geosci, D-28357 Bremen, Germany.
[Hoffmann, Rene] Ruhr Univ Bochum, Inst Geol Mineral & Geophys, Dept Earth Sci, D-44801 Bochum, Germany.
[Fusseis, Florian] Univ Edinburgh, Grant Inst, Sch Geosci, Kings Bldg,West Mains Rd, Edinburgh EH9 3JW, Midlothian, Scotland.
[Ehlke, Moritz; Zachow, Stefan] Zuse Inst Berlin, Dept Visualizat & Data Anal, Med Planning Grp, D-14195 Berlin, Germany.
[Xiao, Xianghui] Argonne Natl Lab, Adv Photon Source, 9700 S Cass Ave, Lemont, IL 60439 USA.
RP Dunlop, JA (reprint author), Leibniz Inst Res Evolut & Biodivers, Museum Nat Kunde, Invalidenstr 43, D-10115 Berlin, Germany.
EM jason.dunlop@mfn-berlin.de
FU U.S. Department of Energy [DE-AC02-06CH11357]; National Institute of
Allergy and Infectious Diseases [R15AI096317]
FX We appreciate technical support by M. Krogmann (Bremen), and thank P.
Selden (Kansas) for useful discussions about fossil arachnids. R.
Garwood and two anonymous reviewers provided valuable comments on the
typescript. Use of the Advanced Photon Source, an Office of Science User
Facility operated for the U.S. Department of Energy (DOE) Office of
Science by Argonne National Laboratory, was supported by the U.S.
Department of Energy under Contract No. DE-AC02-06CH11357. DAA's part of
this project was partially supported by Grant Number R15AI096317 from
the National Institute of Allergy and Infectious Diseases. The content
is the sole responsibility of the authors and does not necessarily
represent the official views of the National Institute of Allergy and
Infectious Diseases or the National Institutes of Health.
NR 57
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Z9 0
U1 3
U2 3
PU BIOMED CENTRAL LTD
PI LONDON
PA 236 GRAYS INN RD, FLOOR 6, LONDON WC1X 8HL, ENGLAND
SN 1471-2148
J9 BMC EVOL BIOL
JI BMC Evol. Biol.
PD OCT 10
PY 2016
VL 16
AR 203
DI 10.1186/s12862-016-0777-y
PG 8
WC Evolutionary Biology; Genetics & Heredity
SC Evolutionary Biology; Genetics & Heredity
GA DZ7DT
UT WOS:000386025400001
PM 27724841
ER
PT J
AU Hell, N
Brown, GV
Wilms, J
Grinberg, V
Clementson, J
Liedahl, D
Porter, FS
Kelley, RL
Kilbourne, CA
Beiersdorfer, P
AF Hell, N.
Brown, G. V.
Wilms, J.
Grinberg, V.
Clementson, J.
Liedahl, D.
Porter, F. S.
Kelley, R. L.
Kilbourne, C. A.
Beiersdorfer, P.
TI LABORATORY MEASUREMENTS OF THE K-SHELL TRANSITION ENERGIES IN L-SHELL
IONS OF SI AND S
SO ASTROPHYSICAL JOURNAL
LA English
DT Article
DE atomic data; methods: laboratory: atomic; X-rays: binaries; X-rays:
general
ID X-RAY SPECTROSCOPY; CHANDRA GRATING SPECTROSCOPY; FLEXIBLE ATOMIC CODE;
HIGHLY-CHARGED IONS; ELECTRON-BEAM; VELA X-1; ABSORPTION-LINES;
CALORIMETER SPECTROMETER; ISOELECTRONIC SEQUENCE; XRS MICROCALORIMETER
AB We have measured the energies of the strongest 1s-2l (l = s, p) transitions in He-through Ne-like silicon and sulfur ions to an accuracy of < 1 eV using the Lawrence Livermore National Laboratory's electron beam ion traps, EBIT-I and SuperEBIT, and the NASA/GSFC EBIT Calorimeter Spectrometer (ECS). We identify and measure the energies of 18 and 21 X-ray features from silicon and sulfur, respectively. The results are compared to new Flexible Atomic Code calculations and to semi-relativistic Hartree-Fock calculations by Palmeri et al. (2008). These results will be especially useful for wind diagnostics in high-mass X-ray binaries, such as Vela X-1 and Cygnus X-1, where high-resolution spectral measurements using Chandra's high-energy transmission grating has made it possible to measure Doppler shifts of 100 km s(-1). The accuracy of our measurements is consistent with that needed to analyze Chandra observations, exceeding Chandra's 100 km s(-1) limit. Hence, the results presented here not only provide benchmarks for theory, but also accurate rest energies that can be used to determine the bulk motion of material in astrophysical sources. We show the usefulness of our results by applying them to redetermine Doppler shifts from Chandra observations of Vela X-1.
C1 [Hell, N.; Wilms, J.] Univ Erlangen Nurnberg, Dr Karl Remeis Sternwarte & Erlangen Ctr Astropar, Sternwartstr 7, D-96049 Bamberg, Germany.
[Hell, N.; Brown, G. V.; Clementson, J.; Liedahl, D.; Beiersdorfer, P.] Lawrence Livermore Natl Lab, 7000 East Ave, Livermore, CA 94550 USA.
[Grinberg, V.] MIT, Kavli Inst Astrophys & Space Res, Cambridge, MA 02139 USA.
[Porter, F. S.; Kelley, R. L.; Kilbourne, C. A.] NASA GSFC, 8800 Greenbelt Rd, Greenbelt, MD 20771 USA.
RP Hell, N (reprint author), Univ Erlangen Nurnberg, Dr Karl Remeis Sternwarte & Erlangen Ctr Astropar, Sternwartstr 7, D-96049 Bamberg, Germany.; Hell, N (reprint author), Lawrence Livermore Natl Lab, 7000 East Ave, Livermore, CA 94550 USA.
EM natalie.hell@sternwarte.uni-erlangen.de
RI Wilms, Joern/C-8116-2013; Porter, Frederick/D-3501-2012
OI Wilms, Joern/0000-0003-2065-5410; Porter, Frederick/0000-0002-6374-1119
FU US DOE [DE-AC52-07NA27344]; NASA [NNX/2AH84G, NAS8-03060];
Bundesministerium fur Wirtschaft und Technologie [DLR 50 OR 1113];
European Space Agency [4000114313/15/NL/CB]; NASA through the
Smithsonian Astrophysical Observatory (SAO) [SV3-73016]
FX This work was performed by LLNL under the auspices of the US DOE under
Contract DE-AC52-07NA27344. It was supported by NASA work orders
NNX/2AH84G; by the Bundesministerium fur Wirtschaft und Technologie
under grant number DLR 50 OR 1113; by the European Space Agency under
contract No. 4000114313/15/NL/CB; and by NASA through the Smithsonian
Astrophysical Observatory (SAO) contract SV3-73016 to MIT for support of
the Chandra X-ray Center (CXC) and Science Instruments. CXC is operated
by SAO for and on the behalf of NASA under contract NAS8-03060. This
research has made use of ISIS functions provided by ECAP/Remeis
observatory and MIT (http://www.sternwarte.uni-erlangen.de/isis/). We
thank John E. Davis for providing the s1xfig module used for creating
the presented plots. CHIANTI is a collaborative project involving George
Mason University, the University of Michigan (USA) and the University of
Cambridge (UK).
NR 81
TC 0
Z9 0
U1 5
U2 5
PU IOP PUBLISHING LTD
PI BRISTOL
PA TEMPLE CIRCUS, TEMPLE WAY, BRISTOL BS1 6BE, ENGLAND
SN 0004-637X
EI 1538-4357
J9 ASTROPHYS J
JI Astrophys. J.
PD OCT 10
PY 2016
VL 830
IS 1
AR 26
DI 10.3847/0004-637X/830/1/26
PG 16
WC Astronomy & Astrophysics
SC Astronomy & Astrophysics
GA DZ1XA
UT WOS:000385633900009
ER
PT J
AU Hollinshead, WD
Rodriguez, S
Martin, HG
Wang, G
Baidoo, EEK
Sale, KL
Keasling, JD
Mukhopadhyay, A
Tang, YJJ
AF Hollinshead, Whitney D.
Rodriguez, Sarah
Martin, Hector Garcia
Wang, George
Baidoo, Edward E. K.
Sale, Kenneth L.
Keasling, Jay D.
Mukhopadhyay, Aindrila
Tang, Yinjie J.
TI Examining Escherichia coli glycolytic pathways, catabolite repression,
and metabolite channeling using Delta pfk mutants
SO BIOTECHNOLOGY FOR BIOFUELS
LA English
DT Article
DE C-13; Channeling; EMP; Metabolic modeling; Synthetic biology; Catabolite
repression; Xylose
ID ENTNER-DOUDOROFF PATHWAY; C-13-METABOLIC FLUX ANALYSIS;
PENTOSE-PHOSPHATE PATHWAY; CENTRAL CARBON METABOLISM; INTRACELLULAR
METABOLITES; FATTY-ACIDS; GLUCOSE; SCALE; COPRODUCTION; RESPONSES
AB Background: Glycolysis breakdowns glucose into essential building blocks and ATP/NAD(P)H for the cell, occupying a central role in its growth and bio-production. Among glycolytic pathways, the Entner Doudoroff pathway (EDP) is a more thermodynamically favorable pathway with fewer enzymatic steps than either the Embden-Meyerhof-Parnas pathway (EMPP) or the oxidative pentose phosphate pathway (OPPP). However, Escherichia coli do not use their native EDP for glucose metabolism.
Results: Overexpression of edd and eda in E. coli to enhance EDP activity resulted in only a small shift in the flux directed through the EDP (similar to 20 % of glycolysis flux). Disrupting the EMPP by phosphofructokinase I (pfkA) knockout increased flux through OPPP (similar to 60 % of glycolysis flux) and the native EDP (similar to 14 % of glycolysis flux), while overexpressing edd and eda in this Delta pfkA mutant directed similar to 70 % of glycolytic flux through the EDP. The downregulation of EMPP via the pfkA deletion significantly decreased the growth rate, while EDP overexpression in the Delta pfkA mutant failed to improve its growth rates due to metabolic burden. However, the reorganization of E. coli glycolytic strategies did reduce glucose catabolite repression. The Delta pfkA mutant in glucose medium was able to cometabolize acetate via the citric acid cycle and gluconeogenesis, while EDP overexpression in the Delta pfkA mutant repressed acetate flux toward gluconeogenesis. Moreover, C-13-pulse experiments in the Delta pfkA mutants showed unsequential labeling dynamics in glycolysis intermediates, possibly suggesting metabolite channeling (metabolites in glycolysis are pass from enzyme to enzyme without fully equilibrating within the cytosol medium).
Conclusions: We engineered E. coli to redistribute its native glycolytic flux. The replacement of EMPP by EDP did not improve E. coli glucose utilization or biomass growth, but alleviated catabolite repression. More importantly, our results supported the hypothesis of channeling in the glycolytic pathways, a potentially overlooked mechanism for regulating glucose catabolism and coutilization of other substrates. The presence of channeling in native pathways, if proven true, would affect synthetic biology applications and metabolic modeling.
C1 [Hollinshead, Whitney D.; Tang, Yinjie J.] Washington Univ, Dept Energy Environm & Chem Engn, St Louis, MO 63130 USA.
[Rodriguez, Sarah] Sandia Natl Labs, Livermore, CA USA.
[Rodriguez, Sarah; Martin, Hector Garcia; Wang, George; Baidoo, Edward E. K.; Sale, Kenneth L.; Keasling, Jay D.; Mukhopadhyay, Aindrila] Joint BioEnergy Inst, Emeryville, CA 94608 USA.
[Martin, Hector Garcia; Wang, George; Baidoo, Edward E. K.; Sale, Kenneth L.; Keasling, Jay D.; Mukhopadhyay, Aindrila] Lawrence Berkeley Natl Lab, Biol Syst & Engn Div, Berkeley, CA 94720 USA.
[Keasling, Jay D.] Univ Calif Berkeley, Calif Inst Quantitat Biosci QB3, Berkeley, CA 94720 USA.
[Keasling, Jay D.] Univ Calif Berkeley, Dept Bioengn, Berkeley, CA 94720 USA.
[Keasling, Jay D.] Univ Calif Berkeley, Dept Chem & Biomol Engn, Berkeley, CA 94720 USA.
[Keasling, Jay D.] Tech Univ Denmark, Novo Nordisk Fdn Ctr Biosustainabil, Kogle Alle, DK-2970 Horsholm, Denmark.
RP Tang, YJJ (reprint author), Washington Univ, Dept Energy Environm & Chem Engn, St Louis, MO 63130 USA.; Mukhopadhyay, A (reprint author), Joint BioEnergy Inst, Emeryville, CA 94608 USA.; Mukhopadhyay, A (reprint author), Lawrence Berkeley Natl Lab, Biol Syst & Engn Div, Berkeley, CA 94720 USA.
EM amukhopadhyay@lbl.gov; yinjie.tang@seas.wustl.edu
RI Garcia Martin, Hector/B-5357-2009
OI Garcia Martin, Hector/0000-0002-4556-9685
FU NSF [DBI 1356669]; DOE-BER [DESC0012722]; Joint BioEnergy Institute by
the US Department of Energy, Office of Science, Office of Biological and
Environmental Research [DE-AC02-05CH11231]; Lawrence Berkeley National
Laboratory; US Department of Energy; DOE Office of Science Graduate
Fellowship [SCGF2015]
FX This work was supported by NSF (DBI 1356669) and DOE-BER (DESC0012722)
given to YJT and by the Joint BioEnergy Institute
(http://www.jbei.org/), which is supported by the US Department of
Energy, Office of Science, Office of Biological and Environmental
Research, through contract DE-AC02-05CH11231 between Lawrence Berkeley
National Laboratory and the US Department of Energy and DOE Office of
Science Graduate Fellowship (SCGF2015) Program to WDH. The United States
Government retains and the publisher, by accepting the article for
publication, acknowledges that the United States Government retains a
non-exclusive, paid-up, irrevocable, worldwide license to publish or
reproduce the published form of this manuscript, or allow others to do
so, for United States Government purposes.
NR 56
TC 1
Z9 1
U1 9
U2 9
PU BIOMED CENTRAL LTD
PI LONDON
PA 236 GRAYS INN RD, FLOOR 6, LONDON WC1X 8HL, ENGLAND
SN 1754-6834
J9 BIOTECHNOL BIOFUELS
JI Biotechnol. Biofuels
PD OCT 10
PY 2016
VL 9
AR 212
DI 10.1186/s13068-016-0630-y
PG 13
WC Biotechnology & Applied Microbiology; Energy & Fuels
SC Biotechnology & Applied Microbiology; Energy & Fuels
GA DZ1DS
UT WOS:000385579700001
PM 27766116
ER
PT J
AU Lischeske, JJ
Crawford, NC
Kuhn, E
Nagle, NJ
Schell, DJ
Tucker, MP
McMillan, JD
Wolfrum, EJ
AF Lischeske, James J.
Crawford, Nathan C.
Kuhn, Erik
Nagle, Nicholas J.
Schell, Daniel J.
Tucker, Melvin P.
McMillan, James D.
Wolfrum, Edward J.
TI Assessing pretreatment reactor scaling through empirical analysis
SO BIOTECHNOLOGY FOR BIOFUELS
LA English
DT Article
DE Biomass; Biofuels; Pretreatment; Enzymatic digestibility
ID DILUTE-ACID PRETREATMENT; LIGNOCELLULOSIC BIOMASS; ENZYMATIC-HYDROLYSIS;
SEVERITY PARAMETER; WHEAT-STRAW; CORN STOVER; TECHNOLOGIES; REACTIVITY;
CELLULOSE; ETHANOL
AB Background: Pretreatment is a critical step in the biochemical conversion of lignocellulosic biomass to fuels and chemicals. Due to the complexity of the physicochemical transformations involved, predictively scaling up technology from bench-to pilot-scale is difficult. This study examines how pretreatment effectiveness under nominally similar reaction conditions is influenced by pretreatment reactor design and scale using four different pretreatment reaction systems ranging from a 3 g batch reactor to a 10 dry-ton/days continuous reactor. The reactor systems examined were an automated solvent extractor (ASE), steam explosion reactor (SER), ZipperClave (R) Reactor (ZCR), and large continuous horizontal screw reactor (LHR). To our knowledge, this is the first such study performed on pretreatment reactors across a range of reaction conditions and at different reactor scales.
Results: The comparative pretreatment performance results obtained for each reactor system were used to develop response surface models for total xylose yield after pretreatment and total sugar yield after pretreatment followed by enzymatic hydrolysis. Near-and very-near-optimal regions were defined as the set of conditions that the model identified as producing yields within one and two standard deviations of the optimum yield. Optimal conditions identified in the smallest scale system (the ASE) were within the near-optimal region of the largest scale reactor system evaluated. The maximum total sugar yields for the ASE and LHR were 95%, while 89% was the optimum observed in the ZipperClave.
Conclusions: The optimum condition identified using the automated and less costly to operate ASE system was within the very-near-optimal space for the total xylose yield of both the ZCR and the LHR, and was within the near-optimal space for total sugar yield for the LHR. This indicates that the ASE is a good tool for cost effectively finding near-optimal conditions for operating pilot-scale systems. Additionally, using a severity factor approach to optimization was found to be inadequate compared to a multivariate optimization method. Finally, the ASE and the LHR were able to enable significantly higher total sugar yields after enzymatic hydrolysis relative to the ZCR, despite having similar optimal conditions and total xylose yields. This underscores the importance of mechanical disruption during pretreatment to improvement of enzymatic digestibility.
C1 [Lischeske, James J.; Crawford, Nathan C.; Kuhn, Erik; Nagle, Nicholas J.; Schell, Daniel J.; Tucker, Melvin P.; McMillan, James D.; Wolfrum, Edward J.] Natl Bioenergy Ctr, Natl Renewable Energy Lab, 15013 Denver West Pkwy, Golden, CO 80401 USA.
RP Lischeske, JJ (reprint author), Natl Bioenergy Ctr, Natl Renewable Energy Lab, 15013 Denver West Pkwy, Golden, CO 80401 USA.
EM james.lischeske@nrel.gov
OI Wolfrum, Edward/0000-0002-7361-8931
FU US Department of Energy [DE-AC36-08GO28308]; National Renewable Energy
Laboratory
FX This work was supported by the US Department of Energy under Contract
No. DE-AC36-08GO28308 with the National Renewable Energy Laboratory.
NR 27
TC 0
Z9 0
U1 7
U2 7
PU BIOMED CENTRAL LTD
PI LONDON
PA 236 GRAYS INN RD, FLOOR 6, LONDON WC1X 8HL, ENGLAND
SN 1754-6834
J9 BIOTECHNOL BIOFUELS
JI Biotechnol. Biofuels
PD OCT 10
PY 2016
VL 9
AR 213
DI 10.1186/s13068-016-0620-0
PG 13
WC Biotechnology & Applied Microbiology; Energy & Fuels
SC Biotechnology & Applied Microbiology; Energy & Fuels
GA DZ1DS
UT WOS:000385579700002
PM 27766117
ER
PT J
AU Zhou, TJ
Turner, AG
Kinter, JL
Wang, B
Qian, Y
Chen, XL
Wu, B
Wang, B
Liu, B
Zou, LW
He, B
AF Zhou, Tianjun
Turner, Andrew G.
Kinter, James L.
Wang, Bin
Qian, Yun
Chen, Xiaolong
Wu, Bo
Wang, Bin
Liu, Bo
Zou, Liwei
He, Bian
TI GMMIP (v1.0) contribution to CMIP6: Global Monsoons Model
Inter-comparison Project
SO GEOSCIENTIFIC MODEL DEVELOPMENT
LA English
DT Article
ID ASIAN SUMMER MONSOON; ATLANTIC MULTIDECADAL OSCILLATION; SEA-SURFACE
TEMPERATURE; INTERANNUAL VARIABILITY; TIBETAN PLATEAU;
NORTHERN-HEMISPHERE; AMERICAN MONSOON; INDIAN-OCEAN; CLIMATE; RAINFALL
AB The Global Monsoons Model Inter-comparison Project (GMMIP) has been endorsed by the panel of Coupled Model Inter-comparison Project (CMIP) as one of the participating model inter-comparison projects (MIPs) in the sixth phase of CMIP (CMIP6). The focus of GMMIP is on monsoon climatology, variability, prediction and projection, which is relevant to four of the "Grand Challenges" proposed by the World Climate Research Programme. At present, 21 international modeling groups are committed to joining GMMIP. This overview paper introduces the motivation behind GMMIP and the scientific questions it intends to answer. Three tiers of experiments, of decreasing priority, are designed to examine (a) model skill in simulating the climatology and interannual-to-multidecadal variability of global monsoons forced by the sea surface temperature during historical climate period; (b) the roles of the Interdecadal Pacific Oscillation and Atlantic Multidecadal Oscillation in driving variations of the global and regional monsoons; and (c) the effects of large orographic terrain on the establishment of the monsoons. The outputs of the CMIP6 Diagnostic, Evaluation and Characterization of Klima experiments (DECK), "historical" simulation and endorsed MIPs will also be used in the diagnostic analysis of GMMIP to give a comprehensive understanding of the roles played by different external forcings, potential improvements in the simulation of monsoon rainfall at high resolution and reproducibility at decadal timescales. The implementation of GMMIP will improve our understanding of the fundamental physics of changes in the global and regional monsoons over the past 140 years and ultimately benefit monsoons prediction and projection in the current century.
C1 [Zhou, Tianjun; Chen, Xiaolong; Wu, Bo; Wang, Bin; Liu, Bo; Zou, Liwei; He, Bian] Chinese Acad Sci, Inst Atmospher Phys, LASG, Beijing 100029, Peoples R China.
[Turner, Andrew G.] Univ Reading, NCAS Climate, Reading, Berks, England.
[Turner, Andrew G.] Univ Reading, Dept Meteorol, Reading, Berks, England.
[Kinter, James L.] George Mason Univ, Ctr Ocean Land Atmosphere Studies, Fairfax, VA 22030 USA.
[Kinter, James L.] George Mason Univ, Dept Atmospher Ocean & Earth Sci, Fairfax, VA 22030 USA.
[Wang, Bin] Univ Hawaii Manoa, Sch Ocean & Earth Sci & Technol, Dept Meteorol, Honolulu, HI USA.
[Qian, Yun] Pacific Northwest Natl Lab, Atmospher Sci & Global Change Div, Richland, WA USA.
[Liu, Bo] Chinese Acad Sci, Grad Univ, Coll Earth Sci, Beijing 100049, Peoples R China.
RP Zhou, TJ (reprint author), Chinese Acad Sci, Inst Atmospher Phys, LASG, Beijing 100029, Peoples R China.
EM zhoutj@lasg.iap.ac.cn
RI Turner, Andrew/D-2286-2009; qian, yun/E-1845-2011; Liu, Bo/M-1151-2015
OI Turner, Andrew/0000-0002-0642-6876; Liu, Bo/0000-0003-3018-7809
FU International Big Science Project - Chinese Academy of Sciences
[134111KYSB20160031]; National Natural Science Foundation of China
[41330423, 41125017]; R&D Special Fund for Public Welfare Industry
(meteorology) [GYHY201506012]; National Centre for Atmospheric Sciences,
Climate Directorate; National Basic Research Program of China
[2014CB441302]; U.S. Department of Energy's Office of Science as part of
the Earth System Modeling Program; DOE [DE-AC05-76RL01830]; China
Postdoctoral Science Foundation [2015M581152]
FX Tianjun Zhou acknowledges the support of International Big Science
Project funded by Chinese Academy of Sciences (no. 134111KYSB20160031),
and National Natural Science Foundation of China under grant nos.
41330423 and 41125017. Bo Wu acknowledges the support of R&D Special
Fund for Public Welfare Industry (meteorology) (GYHY201506012). Andrew
G. Turner acknowledges the support of the National Centre for
Atmospheric Sciences, Climate Directorate. Bin Wang from IAP
acknowledges the support of National Basic Research Program of China
under grant no. 2014CB441302. Yun Qian's contribution is supported by
the U.S. Department of Energy's Office of Science as part of the Earth
System Modeling Program. The Pacific Northwest National Laboratory is
operated for DOE by Battelle Memorial Institute under contract
DE-AC05-76RL01830. Xiaolong Chen acknowledges the support of China
Postdoctoral Science Foundation under grant no. 2015M581152.
NR 80
TC 2
Z9 2
U1 6
U2 6
PU COPERNICUS GESELLSCHAFT MBH
PI GOTTINGEN
PA BAHNHOFSALLEE 1E, GOTTINGEN, 37081, GERMANY
SN 1991-959X
EI 1991-9603
J9 GEOSCI MODEL DEV
JI Geosci. Model Dev.
PD OCT 10
PY 2016
VL 9
IS 10
DI 10.5194/gmd-9-3589-2016
PG 16
WC Geosciences, Multidisciplinary
SC Geology
GA DY8NT
UT WOS:000385387800001
ER
PT J
AU Dumitrescu, E
Humble, TS
AF Dumitrescu, Eugene
Humble, Travis S.
TI Discrimination of correlated and entangling quantum channels with
selective process tomography
SO PHYSICAL REVIEW A
LA English
DT Article
ID ERROR-DETECTION; QUBITS; GATE
AB The accurate and reliable characterization of quantum dynamical processes underlies efforts to validate quantum technologies, where discrimination between competing models of observed behaviors inform efforts to fabricate and operate qubit devices. We present a protocol for quantum channel discrimination that leverages advances in direct characterization of quantum dynamics (DCQD) codes. We demonstrate that DCQD codes enable selective process tomography to improve discrimination between entangling and correlated quantum dynamics. Numerical simulations show selective process tomography requires only a few measurement configurations to achieve a low false alarm rate and that the DCQD encoding improves the resilience of the protocol to hidden sources of noise. Our results show that selective process tomography with DCQD codes is useful for efficiently distinguishing sources of correlated crosstalk from uncorrelated noise in current and future experimental platforms.
C1 [Dumitrescu, Eugene] Oak Ridge Natl Lab, Quantum Comp Inst, Oak Ridge, TN 37831 USA.
Univ Tennessee, Bredesen Ctr Interdisciplinary Res & Grad Educ, Knoxville, TN 37996 USA.
RP Dumitrescu, E (reprint author), Oak Ridge Natl Lab, Quantum Comp Inst, Oak Ridge, TN 37831 USA.
OI Dumitrescu, Eugene/0000-0001-5851-9567
FU Intelligence Community Postdoctoral Research Fellowship program; U.S.
Department of Energy [DE-AC0500OR22725]; Department of Energy; United
States Government
FX This work was supported by a grant from the Intelligence Community
Postdoctoral Research Fellowship program to the University of
Tennessee.; This manuscript has been authored by UT-Battelle, LLC, under
Contract No. DE-AC0500OR22725 with the U.S. Department of Energy. The
United States Government retains and the publisher, by accepting the
article for publication, acknowledges that the United States Government
retains a nonexclusive, paid-up, irrevocable, worldwide license to
publish or reproduce the published form of this manuscript, or allow
others to do so, for the United States Government purposes. The
Department of Energy will provide public access to these results of
federally sponsored research in accordance with the DOE Public Access
Plan.
NR 32
TC 0
Z9 0
U1 2
U2 2
PU AMER PHYSICAL SOC
PI COLLEGE PK
PA ONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA
SN 2469-9926
EI 2469-9934
J9 PHYS REV A
JI Phys. Rev. A
PD OCT 10
PY 2016
VL 94
IS 4
AR 042107
DI 10.1103/PhysRevA.94.042107
PG 12
WC Optics; Physics, Atomic, Molecular & Chemical
SC Optics; Physics
GA DZ1RF
UT WOS:000385616000003
ER
PT J
AU Emmons, SB
Kang, D
Platter, L
AF Emmons, Samuel B.
Kang, Daekyoung
Platter, Lucas
TI Operator product expansion beyond leading order for two-component
fermions
SO PHYSICAL REVIEW A
LA English
DT Article
ID EFFECTIVE-FIELD THEORY; GAS; SCATTERING; ALGEBRA; MODELS
AB We consider a homogeneous, balanced gas of strongly interacting fermions in two spin states interacting through a large scattering length. Finite-range corrections are needed for a quantitative description of data which experiments and numerical simulations have provided. We use a perturbative field-theoretical framework and a tool called the operator product expansion (OPE), which together allow for the expression of finite-range corrections to the universal relations and momentum distribution. By using the OPE, we derive the 1/k(6) part of the momentum tail, which is related to the sum of the derivative of the energy with respect to the finite range and the averaged kinetic energy of opposite spin pairs. By comparing the 1/k(4) term and the 1/k(6) correction in the momentum distribution to provided quantum Monte Carlo (QMC) data, we show that including the 1/k(6) part offers marked improvements. Our field-theoretical approach allows for a clear understanding of the role of the scattering length and finite effective range in the universal relations and the momentum distribution.
C1 [Emmons, Samuel B.] Univ Tennessee, Dept Phys & Astron, Knoxville, TN 37996 USA.
[Kang, Daekyoung] Los Alamos Natl Lab, Theoret Div, MS B283, Los Alamos, NM 87545 USA.
[Platter, Lucas] Oak Ridge Natl Lab, Div Phys, Oak Ridge, TN 37831 USA.
RP Emmons, SB (reprint author), Univ Tennessee, Dept Phys & Astron, Knoxville, TN 37996 USA.
EM semmons@vols.utk.edu; kang1@lanl.gov; lplatter@utk.edu
FU U.S. Department of Energy through the Office of Science, Office of
Nuclear Physics [DE-AC52-06NA25396, DE-AC05-00OR22725]; LANL/LDRD
Program; National Science Foundation [PHY-1516077]; Early Career
Research Award
FX We thank J. Carlson and S. Gandolfi for providing their QMC results and
E. Mereghetti for helpful discussions. We thank E. Braaten for comments
and Y. Castin and F. Werner for their feedback on the manuscript. D.K.
would like to thank the University of Tennessee, Knoxville for
hospitality while this work was started. This work was supported by the
U.S. Department of Energy through the Office of Science, Office of
Nuclear Physics under Contract Nos. DE-AC52-06NA25396,
DE-AC05-00OR22725, an Early Career Research Award, the LANL/LDRD
Program, and by the National Science Foundation under Grant No.
PHY-1516077.
NR 48
TC 1
Z9 1
U1 0
U2 0
PU AMER PHYSICAL SOC
PI COLLEGE PK
PA ONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA
SN 2469-9926
EI 2469-9934
J9 PHYS REV A
JI Phys. Rev. A
PD OCT 10
PY 2016
VL 94
IS 4
AR 043615
DI 10.1103/PhysRevA.94.043615
PG 12
WC Optics; Physics, Atomic, Molecular & Chemical
SC Optics; Physics
GA DZ1RF
UT WOS:000385616000009
ER
PT J
AU Ranjbar, VH
Meot, F
Bai, M
Abell, DT
Meiser, D
AF Ranjbar, V. H.
Meot, F.
Bai, M.
Abell, D. T.
Meiser, D.
TI Polarization response of RHIC electron lens lattices
SO PHYSICAL REVIEW ACCELERATORS AND BEAMS
LA English
DT Article
AB Depolarization response for a system of two orthogonal snakes at irrational tunes is studied in depth using lattice independent spin integration. In particular we consider the effect of overlapping spin resonances in this system, to understand the impact of phase, tune, relative location and threshold strengths of the spin resonances. These results are benchmarked and compared to two dimensional direct tracking results for the RHIC e-lens lattice and the standard lattice. Finally we consider the effect of longitudinal motion via chromatic scans using direct six dimensional lattice tracking.
C1 [Ranjbar, V. H.; Meot, F.] Brookhaven Natl Lab, Upton, NY 11973 USA.
[Bai, M.] Forschungszentrum Julich, D-52428 Julich, Germany.
[Abell, D. T.; Meiser, D.] Tech X Corp, Boulder, CO 80303 USA.
RP Ranjbar, VH (reprint author), Brookhaven Natl Lab, Upton, NY 11973 USA.
EM vranjbar@bnl.gov; fmeot@bnl.gov; m.bai@fz-juelich.de; dabell@txcorp.com;
dmeiser79@gmail.com
FU BNL; U.S. Department of Energy [DE-SC0012704]; U.S. Department of
Energy, Office of Science, Office of Nuclear Physics [DE-SC0004432,
DE-SC0013187]; Office of Science of the U.S. Department of Energy
[DE-AC02-05CH11231, DE-AC05-00OR22725]
FX This work is supported by BNL and the U.S. Department of Energy under
Contract No. DE-SC0012704. It is also supported by the U.S. Department
of Energy, Office of Science, Office of Nuclear Physics, including
Grants No. DE-SC0004432 and No. DE-SC0013187. This research used
resources of the National Energy Research Scientific Computing Center
(NERSC), which is supported by the Office of Science of the U.S.
Department of Energy under Contract No. DE-AC02-05CH11231. This research
also used resources of the Oak Ridge Leadership Computing Facility at
Oak Ridge National Laboratory, which is supported by the Office of
Science of the U.S. Department of Energy under Contract No.
DE-AC05-00OR22725.
NR 18
TC 0
Z9 0
U1 0
U2 0
PU AMER PHYSICAL SOC
PI COLLEGE PK
PA ONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA
SN 2469-9888
J9 PHYS REV ACCEL BEAMS
JI Phys. Rev. Accel. Beams
PD OCT 10
PY 2016
VL 19
IS 10
AR 101002
DI 10.1103/PhysRevAccelBeams.19.101002
PG 13
WC Physics, Nuclear; Physics, Particles & Fields
SC Physics
GA DZ2AC
UT WOS:000385643100001
ER
PT J
AU Koutroulakis, G
Yasuoka, H
Tobash, PH
Mitchell, JN
Bauer, ED
Thompson, JD
AF Koutroulakis, G.
Yasuoka, H.
Tobash, P. H.
Mitchell, J. N.
Bauer, E. D.
Thompson, J. D.
TI Extended nuclear quadrupole resonance study of the heavy-fermion
superconductor PuCoGa5
SO PHYSICAL REVIEW B
LA English
DT Article
ID UNCONVENTIONAL SUPERCONDUCTIVITY; SINGLE-CRYSTAL; METALS; SPIN;
FLUCTUATIONS; RELAXATION; STATES
AB PuCoGa5 has emerged as a prototypical heavy-fermion superconductor, with its transition temperature (T-c similar or equal to 18.5 K) being the highest amongst such materials. Nonetheless, a clear description as to what drives the superconducting pairing is still lacking, rendered complicated by the notoriously intricate nature of plutonium's 5f valence electrons. Here, we present a detailed Ga-69,Ga-71 nuclear quadrupole resonance (NQR) study of PuCoGa5, concentrating on the system's normal state properties near to T-c and aiming to detect distinct signatures of possible pairing mechanisms. In particular, the quadrupole frequency and spin-lattice relaxation rate were measured for the two crystallographically inequivalent Ga sites and for both Ga isotopes, in the temperature range 1.6-300 K. No evidence of significant charge fluctuations is found from the NQR observables. On the contrary, the low-energy dynamics is dominated by anisotropic spin fluctuations with strong, nearly critical, in-plane character, which are effectively identical to the case of the sister compound PuCoIn5. These findings are discussed within the context of different theoretical proposals for the unconventional pairing mechanism in heavy-fermion superconductors.
C1 [Koutroulakis, G.; Yasuoka, H.; Tobash, P. H.; Mitchell, J. N.; Bauer, E. D.; Thompson, J. D.] Los Alamos Natl Lab, Los Alamos, NM 87545 USA.
[Koutroulakis, G.] Univ Calif Los Angeles, Dept Phys, Los Angeles, CA 90095 USA.
RP Koutroulakis, G (reprint author), Los Alamos Natl Lab, Los Alamos, NM 87545 USA.; Koutroulakis, G (reprint author), Univ Calif Los Angeles, Dept Phys, Los Angeles, CA 90095 USA.
OI Mitchell, Jeremy/0000-0001-7109-3505; Bauer, Eric/0000-0003-0017-1937
FU U.S. Department of Energy, Office of Basic Energy Sciences, Division of
Materials Sciences and Engineering; Los Alamos Laboratory Directed
Research and Development program; Glenn T. Seaborg Institute
FX This work was performed under the auspices of the U.S. Department of
Energy, Office of Basic Energy Sciences, Division of Materials Sciences
and Engineering. P.H.T. and J.N.M were supported through the Los Alamos
Laboratory Directed Research and Development program. G.K. and H.Y.
acknowledge support from the Glenn T. Seaborg Institute.
NR 40
TC 0
Z9 0
U1 4
U2 4
PU AMER PHYSICAL SOC
PI COLLEGE PK
PA ONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA
SN 2469-9950
EI 2469-9969
J9 PHYS REV B
JI Phys. Rev. B
PD OCT 10
PY 2016
VL 94
IS 16
AR 165115
DI 10.1103/PhysRevB.94.165115
PG 6
WC Physics, Condensed Matter
SC Physics
GA DZ1UR
UT WOS:000385627000006
ER
PT J
AU Monney, C
Bisogni, V
Zhou, KJ
Kraus, R
Strocov, VN
Behr, G
Drechsler, SL
Rosner, H
Johnston, S
Geck, J
Schmitt, T
AF Monney, Claude
Bisogni, Valentina
Zhou, Ke-Jin
Kraus, Roberto
Strocov, Vladimir N.
Behr, Guenter
Drechsler, Stefan-Ludwig
Rosner, Helge
Johnston, Steve
Geck, Jochen
Schmitt, Thorsten
TI Probing inter- and intrachain Zhang-Rice excitons in Li2CuO2 and
determining their binding energy
SO PHYSICAL REVIEW B
LA English
DT Article
ID X-RAY-SCATTERING; CHAIN CUPRATE LI2CUO2; EXCITATIONS; CRYSTAL;
SPECTROSCOPY; SINGLETS; OXYGEN
AB Cuprate materials, such as those hosting high-temperature superconductivity, represent a famous class of materials where the correlations between the strongly entangled charges and spins produce complex phase diagrams. Several years ago, the Zhang-Rice singlet was proposed as a natural quasiparticle in hole-doped cuprates. The occurrence and binding energy of this quasiparticle, consisting of a pair of bound holes with antiparallel spins on the same CuO4 plaquette, depends on the local electronic interactions, which are fundamental quantities for understanding the physics of the cuprates. Here, we employ state-of-the-art resonant inelastic x-ray scattering (RIXS) to probe the correlated physics of the CuO4 plaquettes in the quasi-one-dimensional chain cuprate Li2CuO2. By tuning the incoming photon energy to the O K edge, we populate bound states related to the Zhang-Rice quasiparticles in the RIXS process. Both intra-and interchain Zhang-Rice singlets are observed and their occurrence is shown to depend on the nearest-neighbor spin-spin correlations, which are readily probed in this experiment. We also extract the binding energy of the Zhang-Rice singlet and identify the Zhang-Rice triplet excitation in the RIXS spectra.
C1 [Monney, Claude; Bisogni, Valentina; Zhou, Ke-Jin; Strocov, Vladimir N.; Schmitt, Thorsten] Paul Scherrer Inst, Res Dept Synchrotron Radiat & Nanotechnol, CH-5232 Villigen, Switzerland.
[Monney, Claude] Univ Zurich, Inst Phys, Winterthurerstr 190, CH-8057 Zurich, Switzerland.
[Bisogni, Valentina] Brookhaven Natl Lab, Natl Synchrotron Light Source 2, Upton, NY 11973 USA.
[Bisogni, Valentina; Kraus, Roberto; Behr, Guenter; Drechsler, Stefan-Ludwig] Leibniz Inst Solid State & Mat Res, Helmholtzstr 20, D-01171 Dresden, Germany.
[Zhou, Ke-Jin] Diamond Light Source, Harwell Sci & Innovat Campus, Didcot OX11 0DE, Oxon, England.
[Rosner, Helge] Max Planck Inst Chem Phys Solids, D-01187 Dresden, Germany.
[Johnston, Steve] Univ Tennessee, Dept Phys & Astron, Knoxville, TN 37996 USA.
[Johnston, Steve] Univ Tennessee, Joint Inst Adv Mat, Knoxville, TN 37996 USA.
[Geck, Jochen] Paris Lodron Univ Salzburg, Chem & Phys Mat, A-5020 Salzburg, Austria.
RP Monney, C (reprint author), Paul Scherrer Inst, Res Dept Synchrotron Radiat & Nanotechnol, CH-5232 Villigen, Switzerland.; Monney, C (reprint author), Univ Zurich, Inst Phys, Winterthurerstr 190, CH-8057 Zurich, Switzerland.
EM monney@physik.uzh.ch; thorsten.schmitt@psi.ch
RI Monney, Claude/C-5553-2011; Schmitt, Thorsten/A-7025-2010
FU Swiss National Science Foundation; National Centre of Competence in
Research MaNEP; German Science Foundation; Swiss National Science
Foundation within the D-A-CH program [200021L_141325, GE 1647/3-1]; SNSF
[PZ00P2_154867]; University of Tennessee's Science Alliance Joint
Directed Research and Development (JDRD) program; Oak Ridge National
Laboratory; Collaborative Research Center [SFB 1143]
FX We acknowledge fruitful discussions with H.M. Ronnow, U. Staub, J. van
der Brink, J. Malek, R. Kuzian, and K. Wohlfeld. S.L.D. thanks A. Boris
and D. Efremov for discussions of the role of interchain ZR excitons.
The experimental part of this work was performed at the ADRESS beam line
of the Swiss Light Source at the Paul Scherrer Institut, Switzerland.
This project was supported by the Swiss National Science Foundation and
its National Centre of Competence in Research MaNEP. This research has
been jointly funded by the German Science Foundation and the Swiss
National Science Foundation within the D-A-CH program (SNSF Grant No.
200021L_141325 and DFG Grant No. GE 1647/3-1). C.M. gratefully
acknowledges the support by the SNSF under Grant No. PZ00P2_154867. S.J.
is supported by the University of Tennessee's Science Alliance Joint
Directed Research and Development (JDRD) program, a collaboration with
Oak Ridge National Laboratory. J.G. gratefully acknowledges the support
by the Collaborative Research Center SFB 1143.
NR 36
TC 0
Z9 0
U1 11
U2 11
PU AMER PHYSICAL SOC
PI COLLEGE PK
PA ONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA
SN 2469-9950
EI 2469-9969
J9 PHYS REV B
JI Phys. Rev. B
PD OCT 10
PY 2016
VL 94
IS 16
AR 165118
DI 10.1103/PhysRevB.94.165118
PG 8
WC Physics, Condensed Matter
SC Physics
GA DZ1UR
UT WOS:000385627000009
ER
PT J
AU Tsvelik, AM
AF Tsvelik, A. M.
TI Fractionalized Fermi liquid in a Kondo-Heisenberg model
SO PHYSICAL REVIEW B
LA English
DT Article
ID CRITICAL-POINT; CUPRATE; DENSITY; STATE; THEOREM
AB The Kondo-Heisenberg model is used as a controllable tool to demonstrate the existence of a peculiar metallic state with unbroken translational symmetry where the Fermi surface volume is not controlled by the total electron density. I use a nonperturbative approach where the strongest interactions are taken into account by means of exact solution, and corrections are controllable. In agreement with the general requirements formulated by T. Senthil et al. [Phys. Rev. Lett. 90, 216403 (2003)], the resulting metallic state represents a fractionalized Fermi liquid where well defined quasiparticles coexist with gapped fractionalized collective excitations. The system undergoes a phase transition to an ordered phase (charge density wave or superconducting), at the transition temperature which is parametrically small in comparison to the quasiparticle Fermi energy.
C1 [Tsvelik, A. M.] Brookhaven Natl Lab, Condensed Matter Phys & Mat Sci Div, Upton, NY 11973 USA.
RP Tsvelik, AM (reprint author), Brookhaven Natl Lab, Condensed Matter Phys & Mat Sci Div, Upton, NY 11973 USA.
FU U.S. Department of Energy (DOE), Division of Condensed Matter Physics
and Materials Science [DE-AC02-98CH10886]
FX I am grateful to A. Chubukov, N. Robinson, T. M. Rice, A.-M. Tremblay,
G. Kotliar, R. M. Konik, P. D. Johnson, and J. Tranquada for interesting
discussions and encouragement. The work was supported by the U.S.
Department of Energy (DOE), Division of Condensed Matter Physics and
Materials Science, under Contract No. DE-AC02-98CH10886.
NR 38
TC 3
Z9 3
U1 1
U2 1
PU AMER PHYSICAL SOC
PI COLLEGE PK
PA ONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA
SN 2469-9950
EI 2469-9969
J9 PHYS REV B
JI Phys. Rev. B
PD OCT 10
PY 2016
VL 94
IS 16
AR 165114
DI 10.1103/PhysRevB.94.165114
PG 8
WC Physics, Condensed Matter
SC Physics
GA DZ1UR
UT WOS:000385627000005
ER
PT J
AU Wysocki, AL
Kutepov, A
Antropov, VP
AF Wysocki, Aleksander L.
Kutepov, Andrey
Antropov, Vladimir P.
TI Strength and scales of itinerant spin fluctuations in 3d paramagnetic
metals
SO PHYSICAL REVIEW B
LA English
DT Article
AB The full spin density fluctuations (SDF) spectra in 3d paramagnetic metals are analyzed from first principles using the linear response technique. Using the calculated complete wave vector and energy dependence of the dynamic spin susceptibility, we obtain the most important, but elusive, characteristic of SDF in solids: on-site spin correlator (SC). We demonstrate that the SDF have a mixed character consisting of interacting collective and single-particle excitations of similar strength spreading continuously over the entire Brillouin zone and a wide energy range up to femtosecond time scales. These excitations cannot be adiabatically separated and their intrinsically multiscale nature should always be taken into account for a proper description of metallic systems. Overall, in all studied systems, despite the lack of local moment, we found a very large SC resulting in an effective fluctuating moment of the order of several Bohr magnetons.
C1 [Wysocki, Aleksander L.; Kutepov, Andrey; Antropov, Vladimir P.] Ames Lab, Ames, IA 50011 USA.
RP Wysocki, AL (reprint author), Ames Lab, Ames, IA 50011 USA.
EM alexwysocki2@gmail.com
FU Critical Materials Institute, an Energy Innovation Hub - U.S. Department
of Energy (DOE); Office of Basic Energy Science, Division of Materials
Science and Engineering; U.S. DOE [DE-AC02-07CH11358]
FX This work was supported by the Critical Materials Institute, an Energy
Innovation Hub funded by the U.S. Department of Energy (DOE). V.P.
acknowledges the support from the Office of Basic Energy Science,
Division of Materials Science and Engineering. The research was
performed at Ames Laboratory, which is operated for the U.S. DOE by Iowa
State University under Contract No. DE-AC02-07CH11358.
NR 27
TC 0
Z9 0
U1 3
U2 3
PU AMER PHYSICAL SOC
PI COLLEGE PK
PA ONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA
SN 2469-9950
EI 2469-9969
J9 PHYS REV B
JI Phys. Rev. B
PD OCT 10
PY 2016
VL 94
IS 14
AR 140405
DI 10.1103/PhysRevB.94.140405
PG 5
WC Physics, Condensed Matter
SC Physics
GA DZ1ST
UT WOS:000385621000002
ER
PT J
AU Zhao, PW
Gandolfi, S
AF Zhao, P. W.
Gandolfi, S.
TI Radii of neutron drops probed via the neutron skin thickness of nuclei
SO PHYSICAL REVIEW C
LA English
DT Article
ID HARTREE-BOGOLIUBOV THEORY; MEAN-FIELD THEORY; R-PROCESS; DENSITY; STATE;
EQUATION; PHYSICS; ENERGY; MATTER
AB Multineutron systems are crucial to understanding the physics of neutron-rich nuclei and neutron stars. Neutron drops, neutrons confined in an external field, are investigated systematically in both nonrelativistic and relativistic density functional theories and with ab initio calculations. We demonstrate a new strong linear correlation, which is universal in the realm of mean-field models, between the rms radii of neutron drops and the neutron skin thickness of Pb-208 and Ca-48, i.e., the difference between the neutron and proton rms radii of a nucleus. Due to its high quality, this correlation can be used to deduce the radii of neutron drops from the measured neutron skin thickness in a model-independent way, and the radii obtained for neutron drops can provide a useful constraint for realistic three-neutron forces. We also present a new correlation between the slope L of the symmetry energy and the radii of neutron drops, and provide the first validation of such a correlation by using density-functional models and ab initio calculations. These newly established correlations, together with more precise measurements of the neutron skin thicknesses of Pb-208 and Ca-48 and/or accurate determinations of L, will have an enduring impact on the understanding of multineutron interactions, neutron-rich nuclei, neutron stars, etc.
C1 [Zhao, P. W.] Argonne Natl Lab, Div Phys, Argonne, IL 60439 USA.
[Gandolfi, S.] Los Alamos Natl Lab, Div Theoret, Los Alamos, NM 87545 USA.
RP Zhao, PW (reprint author), Argonne Natl Lab, Div Phys, Argonne, IL 60439 USA.
RI Zhao, Pengwei/F-9107-2010;
OI Zhao, Pengwei/0000-0001-8243-2381; Gandolfi, Stefano/0000-0002-0430-9035
FU U.S. Department of Energy (DOE), Office of Science, Office of Nuclear
Physics [DE-AC02-06CH11357, DE-AC52-06NA25396]; NUCLEI SciDAC project;
Office of Science of the US Department of Energy [DE-AC02-05CH11231]
FX The authors thank Steven C. Pieper, Robert B. Wiringa, and R. V. F.
Janssens for valuable discussions and careful reading of the manuscript.
This work is supported by U.S. Department of Energy (DOE), Office of
Science, Office of Nuclear Physics, under Contracts No.
DE-AC02-06CH11357 (P.W.Z.) and No. DE-AC52-06NA25396 (S.G.) and by the
NUCLEI SciDAC project (S.G.). Computational resources have been provided
by the Laboratory Computing Resource Center at Argonne National
Laboratory and by Los Alamos Open Supercomputing. This research used
resources of the National Energy Research Scientific Computing Center, a
DOE Office of Science User Facility supported by the Office of Science
of the US Department of Energy under Contract No. DE-AC02-05CH11231.
NR 65
TC 0
Z9 0
U1 2
U2 2
PU AMER PHYSICAL SOC
PI COLLEGE PK
PA ONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA
SN 2469-9985
EI 2469-9993
J9 PHYS REV C
JI Phys. Rev. C
PD OCT 10
PY 2016
VL 94
IS 4
AR 041302
DI 10.1103/PhysRevC.94.041302
PG 6
WC Physics, Nuclear
SC Physics
GA DZ1VK
UT WOS:000385629200001
ER
PT J
AU Boughezal, R
Liu, XH
Petriello, F
AF Boughezal, Radja
Liu, Xiaohui
Petriello, Frank
TI Phenomenology of the Z boson plus jet process at NNLO
SO PHYSICAL REVIEW D
LA English
DT Article
ID MCFM; LHC
AB We present a detailed phenomenological study of Z-boson production in association with a jet through next-to-next-to-leading order (NNLO) in perturbative QCD. Fiducial cross sections and differential distributions for both 8 TeV and 13 TeV LHC collisions are presented. We study the impact of different parton distribution functions (PDFs) on predictions for the Z + jet process. Upon inclusion of the NNLO corrections, the residual scale uncertainty is reduced such that both the total rate and the transverse momentum distributions can be used to discriminate between various PDF sets.
C1 [Boughezal, Radja] Argonne Natl Lab, Div High Energy Phys, Argonne, IL 60439 USA.
[Liu, Xiaohui] Univ Maryland, Maryland Ctr Fundamental Phys, College Pk, MD 20742 USA.
[Petriello, Frank] Argonne Natl Lab, Div High Energy Phys, Argonne, IL 60439 USA.
[Petriello, Frank] Northwestern Univ, Dept Phys & Astron, Evanston, IL 60208 USA.
RP Boughezal, R (reprint author), Argonne Natl Lab, Div High Energy Phys, Argonne, IL 60439 USA.; Liu, XH (reprint author), Univ Maryland, Maryland Ctr Fundamental Phys, College Pk, MD 20742 USA.; Petriello, F (reprint author), Argonne Natl Lab, Div High Energy Phys, Argonne, IL 60439 USA.; Petriello, F (reprint author), Northwestern Univ, Dept Phys & Astron, Evanston, IL 60208 USA.
EM rboughezal@anl.gov; xhliu@umd.edu; f-petriello@northwestern.edu
FU DOE [DE-AC02-06CH11357, DE-FG02-93ER-40762, DE-FG02-91ER40684]; Office
of Science of the U.S. Department of Energy [DE-AC02-05CH11231]; DOE
Office of Science [DE-AC02-06CH11357]
FX We thank T. LeCompte for helpful discussions. R. B. is supported by DOE
Contract No. DE-AC02-06CH11357. X. L. is supported by DOE Grant No.
DE-FG02-93ER-40762. F. P. is supported by DOE Grants No.
DE-FG02-91ER40684 and No. DE-AC02-06CH11357. This research used
resources of the National Energy Research Scientific Computing Center, a
DOE Office of Science User Facility supported by the Office of Science
of the U.S. Department of Energy under Contract No. DE-AC02-05CH11231.
It also used resources of the Argonne Leadership Computing Facility,
which is a DOE Office of Science User Facility supported under Contract
No. DE-AC02-06CH11357.
NR 35
TC 1
Z9 1
U1 1
U2 1
PU AMER PHYSICAL SOC
PI COLLEGE PK
PA ONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA
SN 2470-0010
EI 2470-0029
J9 PHYS REV D
JI Phys. Rev. D
PD OCT 10
PY 2016
VL 94
IS 7
AR 074015
DI 10.1103/PhysRevD.94.074015
PG 9
WC Astronomy & Astrophysics; Physics, Particles & Fields
SC Astronomy & Astrophysics; Physics
GA DZ1WH
UT WOS:000385631800004
ER
PT J
AU Bellesia, G
Bales, BB
AF Bellesia, Giovanni
Bales, Benjamin B.
TI Population dynamics, information transfer, and spatial organization in a
chemical reaction network under spatial confinement and crowding
conditions
SO PHYSICAL REVIEW E
LA English
DT Article
ID SEMISYNTHETIC MINIMAL CELLS; LIFE; FLUCTUATIONS; DIFFUSION; ORIGIN;
ENTROPY; SYSTEMS; VOLUME; CHAOS; OSCILLATIONS
AB We investigate, via Brownian dynamics simulations, the reaction dynamics of a generic, nonlinear chemical network under spatial confinement and crowding conditions. In detail, theWillamowski-Rossler chemical reaction system has been "extended" and considered as a prototype reaction-diffusion system. Our results are potentially relevant to a number of open problems in biophysics and biochemistry, such as the synthesis of primitive cellular units (protocells) and the definition of their role in the chemical origin of life and the characterization of vesicle-mediated drug delivery processes. More generally, the computational approach presented in this work makes the case for the use of spatial stochastic simulation methods for the study of biochemical networks in vivo where the "well-mixed" approximation is invalid and both thermal and intrinsic fluctuations linked to the possible presence of molecular species in low number copies cannot be averaged out.
C1 [Bellesia, Giovanni] Los Alamos Natl Lab, Theoret Biol & Biophys Grp, Los Alamos, NM 87545 USA.
[Bales, Benjamin B.] Univ Calif Santa Barbara, Dept Comp Sci, Santa Barbara, CA 93106 USA.
RP Bellesia, G (reprint author), Los Alamos Natl Lab, Theoret Biol & Biophys Grp, Los Alamos, NM 87545 USA.
EM giovanni.bellesia@gmail.com
FU NIH [1R01EB014877-01]
FX The authors would like to thank Linda Petzold, Zachary Frazier, Frank
Alber, Marco J. Morelli, and Steve Plimpton for useful discussions and
for the help with the testing of our Brownian simulator. This work has
been supported by NIH Grant No. 1R01EB014877-01.
NR 71
TC 0
Z9 0
U1 7
U2 7
PU AMER PHYSICAL SOC
PI COLLEGE PK
PA ONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA
SN 2470-0045
EI 2470-0053
J9 PHYS REV E
JI Phys. Rev. E
PD OCT 10
PY 2016
VL 94
IS 4
AR 042306
DI 10.1103/PhysRevE.94.042306
PG 8
WC Physics, Fluids & Plasmas; Physics, Mathematical
SC Physics
GA DZ1XK
UT WOS:000385635100005
PM 27841639
ER
PT J
AU Crawford, A
Thomsen, E
Reed, D
Stephenson, D
Sprenkle, V
Liu, J
Viswanathan, V
AF Crawford, Alasdair
Thomsen, Edwin
Reed, David
Stephenson, David
Sprenkle, Vincent
Liu, Jun
Viswanathan, Vilayanur
TI Development and validation of chemistry agnostic flow battery cost
performance model and application to nonaqueous electrolyte systems
SO INTERNATIONAL JOURNAL OF ENERGY RESEARCH
LA English
DT Article
DE nonaqueous; inter-digitated; flow; stack; electrolyte; conductivity
ID IONIC-CONDUCTIVITY; ENERGY-STORAGE; MEMBRANES
AB A chemistry agnostic cost performance model is described for a nonaqueous flow battery. The model predicts flow battery performance by estimating the active reaction zone thickness at each electrode as a function of current density, state of charge, and flow rate using measured data for electrode kinetics, electrolyte conductivity, and electrode-specific surface area. Validation of the model is conducted using a 4kW stack data at various current densities and flow rates. This model is used to estimate the performance of a nonaqueous flow battery with electrode and electrolyte properties used from the literature. The optimized cost for this system is estimated for various power and energy levels using component costs provided by vendors. The model allows optimization of design parameters such as electrode thickness, area, flow path design, and operating parameters such as power density, flow rate, and operating SOC range for various application duty cycles. A parametric analysis is done to identify components and electrode/electrolyte properties with the highest impact on system cost for various application durations. A pathway to 100$ kW h(-1) for the storage system is identified. Copyright (C) 2016 John Wiley & Sons, Ltd.
C1 [Crawford, Alasdair; Thomsen, Edwin; Reed, David; Stephenson, David; Sprenkle, Vincent; Liu, Jun; Viswanathan, Vilayanur] PNNL, 902 Battelle Blvd,POB 999, Richland, WA 99352 USA.
RP Viswanathan, V (reprint author), PNNL, 902 Battelle Blvd,POB 999, Richland, WA 99352 USA.
EM vilayanur.viswanathan@pnl.gov
FU Joint Center for Energy Storage Research, an Energy Innovation Hub - US
Department of Energy, Office of Science, Basic Energy Sciences [63076];
US Department of Energy, Office of Electricity Delivery and Energy
Reliability [57558]; DOE [DE-AC05-76RLO1830]
FX This work was partially funded by the Joint Center for Energy Storage
Research (contract 63076), an Energy Innovation Hub funded by the US
Department of Energy, Office of Science, Basic Energy Sciences.
Additional support was provided by the US Department of Energy, Office
of Electricity Delivery and Energy Reliability (contract 57558). We are
highly appreciative of the guidance provided by Dr Kevin Gallagher of
the Argonne National Laboratory, and the stimulating discussions with Dr
Larry Pederson of PNNL on the challenges facing nonaqueous flow systems.
We acknowledge Prof. Levi Thomson from the University of Michigan for
providing conductivity data for various nonaqueous solvents with
different supporting salts, and also pointing out the possibility of
extracting multiple electrons from each mole of the reactant. The
kinetic rate constant measurements provided by Dr Emily Carino of Prof.
Fikile Brushett's group at MIT are also acknowledged. We appreciate Dr
Xiaoliang Wei of PNNL for providing us preliminary test data for
nonaqueous flow cell. PNNL is operated by Battelle for the DOE under
contract DE-AC05-76RLO1830.
NR 32
TC 0
Z9 0
U1 2
U2 2
PU WILEY-BLACKWELL
PI HOBOKEN
PA 111 RIVER ST, HOBOKEN 07030-5774, NJ USA
SN 0363-907X
EI 1099-114X
J9 INT J ENERG RES
JI Int. J. Energy Res.
PD OCT 10
PY 2016
VL 40
IS 12
BP 1611
EP 1623
DI 10.1002/er.3526
PG 13
WC Energy & Fuels; Nuclear Science & Technology
SC Energy & Fuels; Nuclear Science & Technology
GA DY3CD
UT WOS:000384967500002
ER
PT J
AU Tak, T
Zheng, Y
Lee, D
Kim, TK
AF Tak, Taewoo
Zheng, Youqi
Lee, Deokjung
Kim, T. K.
TI Power flattening study of ultra-long cycle fast reactor using thorium
fuel
SO INTERNATIONAL JOURNAL OF ENERGY RESEARCH
LA English
DT Article
DE ultra-long cycle fast reactor; power flattening; thorium; fuel zoning
ID WEAPON GRADE PLUTONIUM; CANDU REACTOR; BURN-UP; CORE; SUSTAINABILITY;
DESIGN; BUNDLE; CODE
AB This paper presents a design study of power shape flattening for an optimized ultra-long cycle fast reactor with a power rate of 1000 MWe in order to mitigate the power peaking issue and improve the safety with a lower maximum neutron flux and reactivity swing. There are variations in the core designs by loading thorium fuel or zoning fuels in the blanket region and the bottom driver region of ultra-long cycle fast reactor with a power rate of 1000 MWe. While it has lower breeding performance in a fast breeder reactor, thorium fuel is one of the promising fuel options for future reactors because of its abundance and its safety characteristics. It has been confirmed that the thorium fuels, when loaded into the center region of a reactor core, lower the power peaking factor from 1.64 to 1.25 after 20 years and achieves a more flattened radial power distribution. This consequently reduces the maximum neutron flux and the speed of the active core moving from 3.0 cm/year to 2.5 cm/year on the average over the 60-year reactor operation. It has been successfully demonstrated that the three-zone core is the most optimized core, has the most flattened radial power shape, and is without any compromise in the nature of long cycle core, from the neutronics point of view, in terms of average discharge burnup and breeding ratio. Copyright (C) 2016 John Wiley & Sons, Ltd.
C1 [Tak, Taewoo; Zheng, Youqi; Lee, Deokjung] Ulsan Natl Inst Sci & Technol, 50 UNIST Gil, Ulsan 44919, South Korea.
[Kim, T. K.] Argonne Natl Lab, 9700 South Cass Ave, Argonne, IL 60564 USA.
RP Lee, D (reprint author), Ulsan Natl Inst Sci & Technol, 50 UNIST Gil, Ulsan 44919, South Korea.
EM deokjung@unist.ac.kr
OI Lee, Deokjung/0000-0002-3935-5058; Tak, Taewoo/0000-0002-3230-8080
FU National Research Foundation of Korea (NRF) - Korea government (MSIP)
[NRF-2013M2A8A2078243]
FX This work was supported by National Research Foundation of Korea (NRF)
grant funded by the Korea government (MSIP) (no. NRF-2013M2A8A2078243).
NR 34
TC 0
Z9 0
U1 0
U2 0
PU WILEY-BLACKWELL
PI HOBOKEN
PA 111 RIVER ST, HOBOKEN 07030-5774, NJ USA
SN 0363-907X
EI 1099-114X
J9 INT J ENERG RES
JI Int. J. Energy Res.
PD OCT 10
PY 2016
VL 40
IS 12
BP 1662
EP 1672
DI 10.1002/er.3552
PG 11
WC Energy & Fuels; Nuclear Science & Technology
SC Energy & Fuels; Nuclear Science & Technology
GA DY3CD
UT WOS:000384967500006
ER
PT J
AU Hong, WC
Ku, CJ
Li, R
Abbaslou, S
Reyes, P
Wang, SY
Li, GY
Lu, M
Sheng, K
Lu, YC
AF Hong, Wen-Chiang
Ku, Chieh-Jen
Li, Rui
Abbaslou, Siamak
Reyes, Pavel
Wang, Szu-Ying
Li, Guangyuan
Lu, Ming
Sheng, Kuang
Lu, Yicheng
TI MgZnO High Voltage Thin Film Transistors on Glass for Inverters in
Building Integrated Photovoltaics
SO SCIENTIFIC REPORTS
LA English
DT Article
ID RADIATION HARDNESS; SOLAR-CELLS; FABRICATION; POWER
AB Building integrated photovoltaics (BIPV) have attracted considerable interests because of its aesthetically attractive appearance and overall low cost. In BIPV, system integration on a glass substrate like windows is essential to cover a large area of a building with low cost. However, the conventional high voltage devices in inverters have to be built on the specially selected single crystal substrates, limiting its application for large area electronic systems, such as the BIPV. We demonstrate a Magnesium Zinc Oxide (MZO) based high voltage thin film transistor (HVTFT) built on a transparent glass substrate. The devices are designed with unique ring-type structures and use modulated Mg doping in the channel - gate dielectric interface, resulting in a blocking voltage of over 600 V. In addition to BIPV, the MZO HVTFT based inverter technology also creates new opportunities for emerging self-powered smart glass.
C1 [Hong, Wen-Chiang; Ku, Chieh-Jen; Li, Rui; Abbaslou, Siamak; Reyes, Pavel; Wang, Szu-Ying; Li, Guangyuan; Sheng, Kuang; Lu, Yicheng] Rutgers State Univ, Dept Elect & Comp Engn, Piscataway, NJ 08854 USA.
[Lu, Ming] Brookhaven Natl Lab, Ctr Funct Nanomat, Upton, NY 11973 USA.
[Sheng, Kuang] Zhejiang Univ, Coll Elect Engn, Hangzhou 310027, Zhejiang, Peoples R China.
RP Lu, YC (reprint author), Rutgers State Univ, Dept Elect & Comp Engn, Piscataway, NJ 08854 USA.
EM ylu@rci.rutgers.edu
FU National Science Foundation [CBET-1264508]; US Department of Energy,
Office of Basic Energy Sciences [DE-SC0012704]
FX This work was partially supported by the National Science Foundation
under Grant No. CBET-1264508. The research was conducted (in part) at
the Center for Functional Nanomaterials, Brookhaven National Laboratory,
which was supported by the US Department of Energy, Office of Basic
Energy Sciences, under Contract No. DE-SC0012704.
NR 35
TC 0
Z9 0
U1 15
U2 15
PU NATURE PUBLISHING GROUP
PI LONDON
PA MACMILLAN BUILDING, 4 CRINAN ST, LONDON N1 9XW, ENGLAND
SN 2045-2322
J9 SCI REP-UK
JI Sci Rep
PD OCT 10
PY 2016
VL 6
AR 34169
DI 10.1038/srep34169
PG 9
WC Multidisciplinary Sciences
SC Science & Technology - Other Topics
GA DY2KZ
UT WOS:000384922800001
PM 27721484
ER
PT J
AU Jiang, ZH
Dong, XB
Li, ZG
He, F
Zhang, ZD
AF Jiang, Zhenhong
Dong, Xiaobao
Li, Zhi-Gang
He, Fei
Zhang, Ziding
TI Differential Coexpression Analysis Reveals Extensive Rewiring of
Arabidopsis Gene Coexpression in Response to Pseudomonas syringae
Infection
SO SCIENTIFIC REPORTS
LA English
DT Article
ID PLANT IMMUNITY; TRANSCRIPTION FACTORS; BIOLOGICAL NETWORKS; EXPRESSION
PROFILES; DEFENSE RESPONSES; MICROARRAY DATA; MODULES; MECHANISMS;
DYNAMICS; TOMATO
AB Plant defense responses to pathogens involve massive transcriptional reprogramming. Recently, differential coexpression analysis has been developed to study the rewiring of gene networks through microarray data, which is becoming an important complement to traditional differential expression analysis. Using time-series microarray data of Arabidopsis thaliana infected with Pseudomonas syringae, we analyzed Arabidopsis defense responses to P. syringae through differential coexpression analysis. Overall, we found that differential coexpression was a common phenomenon of plant immunity. Genes that were frequently involved in differential coexpression tend to be related to plant immune responses. Importantly, many of those genes have similar average expression levels between normal plant growth and pathogen infection but have different coexpression partners. By integrating the Arabidopsis regulatory network into our analysis, we identified several transcription factors that may be regulators of differential coexpression during plant immune responses. We also observed extensive differential coexpression between genes within the same metabolic pathways. Several metabolic pathways, such as photosynthesis light reactions, exhibited significant changes in expression correlation between normal growth and pathogen infection. Taken together, differential coexpression analysis provides a new strategy for analyzing transcriptional data related to plant defense responses and new insights into the understanding of plant-pathogen interactions.
C1 [Jiang, Zhenhong; Dong, Xiaobao; Li, Zhi-Gang; He, Fei; Zhang, Ziding] China Agr Univ, Coll Biol Sci, State Key Lab Agrobiotechnol, Beijing 100193, Peoples R China.
[He, Fei] Brookhaven Natl Lab, Dept Biol, Upton, NY 11973 USA.
RP He, F; Zhang, ZD (reprint author), China Agr Univ, Coll Biol Sci, State Key Lab Agrobiotechnol, Beijing 100193, Peoples R China.; He, F (reprint author), Brookhaven Natl Lab, Dept Biol, Upton, NY 11973 USA.
EM plane83@gmail.com; zidingzhang@cau.edu.cn
RI Zhang, Ziding/E-9320-2011;
OI Zhang, Ziding/0000-0002-9296-571X; He, Fei/0000-0002-1165-3248
FU National Natural Science Foundation of China [31271414, 31471249]
FX We thank Drs. Saijun Tang, Xiangfeng Wang, and Yuan Zhou at China
Agricultural University for their helpful discussions on this topic.
This work was supported by grants from the National Natural Science
Foundation of China (31271414, 31471249).
NR 68
TC 0
Z9 0
U1 17
U2 17
PU NATURE PUBLISHING GROUP
PI LONDON
PA MACMILLAN BUILDING, 4 CRINAN ST, LONDON N1 9XW, ENGLAND
SN 2045-2322
J9 SCI REP-UK
JI Sci Rep
PD OCT 10
PY 2016
VL 6
AR 35064
DI 10.1038/srep35064
PG 13
WC Multidisciplinary Sciences
SC Science & Technology - Other Topics
GA DY2BR
UT WOS:000384898600001
PM 27721457
ER
PT J
AU Li, WD
Gao, YF
Bei, HB
AF Li, Weidong
Gao, Yanfei
Bei, Hongbin
TI Instability Analysis and Free Volume Simulations of Shear Band
Directions and Arrangements in Notched Metallic Glasses
SO SCIENTIFIC REPORTS
LA English
DT Article
ID DISTRIBUTED WEAK ZONES; MODE FRACTURE; LOCALIZATION; DEFORMATION; FLOW;
CAVITATION; MECHANISM; EVOLUTION; FAILURE; ORIGIN
AB As a commonly used method to enhance the ductility in bulk metallic glasses (BMGs), the introduction of geometric constraints blocks and confines the propagation of the shear bands, reduces the degree of plastic strain on each shear band so that the catastrophic failure is prevented or delayed, and promotes the formation of multiple shear bands. The clustering of multiple shear bands near notches is often interpreted as the reason for improved ductility. Experimental works on the shear band arrangements in notched metallic glasses have been extensively carried out, but a systematic theoretical study is lacking. Using instability theory that predicts the onset of strain localization and the free-volumebased finite element simulations that predict the evolution of shear bands, this work reveals various categories of shear band arrangements in double edge notched BMGs with respect to the mode mixity of the applied stress fields. A mechanistic explanation is thus provided to a number of related experiments and especially the correlation between various types of shear bands and the stress state.
C1 [Li, Weidong; Gao, Yanfei] Univ Tennessee, Dept Mat Sci & Engn, Knoxville, TN 37996 USA.
[Gao, Yanfei; Bei, Hongbin] Oak Ridge Natl Lab, Mat Sci & Technol Div, Oak Ridge, TN 37831 USA.
RP Gao, YF (reprint author), Univ Tennessee, Dept Mat Sci & Engn, Knoxville, TN 37996 USA.; Gao, YF; Bei, HB (reprint author), Oak Ridge Natl Lab, Mat Sci & Technol Div, Oak Ridge, TN 37831 USA.
EM ygao7@utk.edu; beih@ornl.gov
RI Gao, Yanfei/F-9034-2010;
OI Gao, Yanfei/0000-0003-2082-857X; Bei, Hongbin/0000-0003-0283-7990
FU U.S. Department of Energy, Office of Science, Basic Energy Sciences,
Materials Sciences and Engineering Division
FX This research was supported by the U.S. Department of Energy, Office of
Science, Basic Energy Sciences, Materials Sciences and Engineering
Division.
NR 32
TC 1
Z9 1
U1 18
U2 18
PU NATURE PUBLISHING GROUP
PI LONDON
PA MACMILLAN BUILDING, 4 CRINAN ST, LONDON N1 9XW, ENGLAND
SN 2045-2322
J9 SCI REP-UK
JI Sci Rep
PD OCT 10
PY 2016
VL 6
AR 34878
DI 10.1038/srep34878
PG 11
WC Multidisciplinary Sciences
SC Science & Technology - Other Topics
GA DY5NC
UT WOS:000385145500001
PM 27721462
ER
PT J
AU Sawaya, MR
Verma, M
Balendiran, V
Rath, NP
Cascio, D
Balendiran, GK
AF Sawaya, Michael R.
Verma, Malkhey
Balendiran, Vaishnavi
Rath, Nigam P.
Cascio, Duilio
Balendiran, Ganesaratnam K.
TI Characterization of WY 14,643 and its Complex with Aldose Reductase
SO SCIENTIFIC REPORTS
LA English
DT Article
ID CRYSTAL-STRUCTURE; DIABETIC COMPLICATIONS; ACYL GLUCURONIDES; CATALYTIC
SUBUNIT; ALPHA ACTIVATION; LIGAND-BINDING; MECHANISM; FLUORESCENCE;
INHIBITOR; METABOLISM
AB The peroxisome proliferator, WY 14,643 exhibits a pure non-competitive inhibition pattern in the aldehyde reduction and in alcohol oxidation activities of human Aldose reductase (hAR). Fluorescence emission measurements of the equilibrium dissociation constants, K-d, of oxidized (hAR.NADP+) and reduced (hAR.NADPH) holoenzyme complexes display a 2-fold difference between them. Kd values for the dissociation of WY 14,643 from the oxidized (hAR.NADP+.WY 14,643) and reduced (hAR.NADPH.WY 14,643) ternary complexes are comparable to each other. The ternary complex structure of hAR.NADP+.WY 14,643 reveals the first structural evidence of a fibrate class drug binding to hAR. These observations demonstrate how fibrate molecules such as WY 14,643, besides being valued as agonists for PPAR, also inhibit hAR.
C1 [Sawaya, Michael R.; Cascio, Duilio] Univ Calif Los Angeles, US DOE, 611 Charles E Young Dr East,220 Boyer Hall, Los Angeles, CA 90095 USA.
[Verma, Malkhey] Univ Manchester, Manchester Interdisciplinary Bioctr, 131 Princess St, Manchester M1 7DN, Lancs, England.
[Balendiran, Vaishnavi; Balendiran, Ganesaratnam K.] Youngstown State Univ, Dept Chem, WBSH 6017,One Univ Plaza, Youngstown, OH 44555 USA.
[Rath, Nigam P.] Univ Missouri, Dept Chem & Biochem, St Louis, MO 63121 USA.
[Verma, Malkhey] Cent Univ Punjab, Ctr Biochem & Microbial Sci, Bathinda 151001, India.
RP Balendiran, GK (reprint author), Youngstown State Univ, Dept Chem, WBSH 6017,One Univ Plaza, Youngstown, OH 44555 USA.
EM pl_note@yahoo.com
FU National Institutes of Health; Office of Biological and Environmental
Research, U.S. Department of Energy; National Institutes of Health,
National Center for Research Resources, Biomedical; National Institute
of General Medical Sciences
FX This work is supported by National Institutes of Health Grant. We thank
David Eisenberg and Todd Yeates for the use of their facilities; the
staff at SSRL beamline 9-2 for their expert assistance; Dino Moras and
Alberto Podjarny for the gift of the recombinant hAR overexpression
cells. Data collection facilities at the Stanford Synchrotron Radiation
Laboratory (SSRL) are funded by The Office of Biological and
Environmental Research, U.S. Department of Energy, the National
Institutes of Health, National Center for Research Resources,
Biomedical, and the National Institute of General Medical Sciences.
NR 58
TC 0
Z9 0
U1 3
U2 3
PU NATURE PUBLISHING GROUP
PI LONDON
PA MACMILLAN BUILDING, 4 CRINAN ST, LONDON N1 9XW, ENGLAND
SN 2045-2322
J9 SCI REP-UK
JI Sci Rep
PD OCT 10
PY 2016
VL 6
AR 34394
DI 10.1038/srep34394
PG 14
WC Multidisciplinary Sciences
SC Science & Technology - Other Topics
GA DY2LJ
UT WOS:000384923800001
PM 27721416
ER
PT J
AU Yang, XL
Hong, JR
Barone, M
Sotiropoulos, F
AF Yang, Xiaolei
Hong, Jiarong
Barone, Matthew
Sotiropoulos, Fotis
TI Coherent dynamics in the rotor tip shear layer of utility-scale wind
turbines
SO JOURNAL OF FLUID MECHANICS
LA English
DT Article
DE shear layer turbulence; vortex instability; wakes
ID LINEAR-STABILITY ANALYSIS; MEXICO ROTOR; AXIAL-FLOW; WAKE; INSTABILITY;
VORTICES; MODEL; VORTEX; SIMULATION
AB Recent field experiments conducted in the near wake (up to 0.5 rotor diameters downwind of the rotor) of a Clipper Liberty C96 2.5 MW wind turbine using snow-based super-large-scale particle image velocimetry (SLPIV) (Hong et al., Nat. Commun., vol. 5, 2014, 4216) were successful in visualizing tip vortex cores as areas devoid of snowflakes. The so-visualized snow voids, however, suggested tip vortex cores of complex shape consisting of circular cores with distinct elongated comet-like tails. We employ large-eddy simulation (LES) to elucidate the structure and dynamics of the complex tip vortices identified experimentally. We show that the LES, with inflow conditions representing as closely as possible the state of the flow approaching the turbine when the SLPIV experiments were carried out, reproduce vortex cores in good qualitative agreement with the SLPIV results, essentially capturing all vortex core patterns observed in the field in the tip shear layer. The computed results show that the visualized vortex patterns are formed by the tip vortices and a second set of counter-rotating spiral vortices intertwined with the tip vortices. To probe the dependence of these newly uncovered coherent flow structures on turbine design, size and approach flow conditions, we carry out LES for three additional turbines: (i) the Scaled Wind Farm Technology (SWiFT) turbine developed by Sandia National Laboratories in Lubbock, TX, USA; (ii) the wind turbine developed for the European collaborative MEXICO (Model Experiments in Controlled Conditions) project; and (iii) the model turbine presented in the paper by Lignarolo et al. (J. Fluid Mech., vol. 781, 2015, pp. 467-493), and the Clipper turbine under varying inflow turbulence conditions. We show that similar counter-rotating vortex structures as those observed for the Clipper turbine are also observed for the SWiFT, MEXICO and model wind turbines. However, the strength of the counter-rotating vortices relative to that of the tip vortices from the model turbine is significantly weaker. We also show that incoming flows with low level turbulence attenuate the elongation of the tip and counter-rotating vortices. Sufficiently high turbulence levels in the incoming flow, on the other hand, tend to break up the coherence of spiral vortices in the near wake. To elucidate the physical mechanism that gives rise to such rich coherent dynamics we examine the stability of the turbine tip shear layer using the theory proposed by Leibovich & Stewartson (J. Fluid Mech., vol. 126, 1983, pp. 335-356). We show that for all simulated cases the theory consistently indicates the flow to be unstable exactly in the region where counter-rotating spirals emerge. We thus postulate that centrifugal instability of the rotating turbine tip shear layer is a possible mechanism for explaining the phenomena we have uncovered herein.
C1 [Yang, Xiaolei; Hong, Jiarong] Univ Minnesota, St Anthony Falls Lab, 2 Third Ave SE, Minneapolis, MN 55414 USA.
[Hong, Jiarong] Univ Minnesota, Dept Mech Engn, 111 Church St SE, Minneapolis, MN 55455 USA.
[Barone, Matthew] Sandia Natl Labs, POB 5800, Albuquerque, NM 87185 USA.
[Barone, Matthew] Sandia Natl Labs, Livermore, CA 94550 USA.
[Sotiropoulos, Fotis] SUNY Stony Brook, Coll Engn & Appl Sci, Dept Civil Engn, Stony Brook, NY 11794 USA.
RP Sotiropoulos, F (reprint author), SUNY Stony Brook, Coll Engn & Appl Sci, Dept Civil Engn, Stony Brook, NY 11794 USA.
EM fotis.sotiropoulos@stonybrook.edu
FU Department of Energy DOE [DE-EE0002980, DE-EE0005482,
DE-AC04-94AL85000]; Sandia National Laboratories [DE-AC04-94AL85000];
Renewable Development Fund [RD4-13]; NSF Career Award [NSF-CBET-1454259]
FX This work was supported by Department of Energy DOE (DE-EE0002980,
DE-EE0005482 and DE-AC04-94AL85000), Sandia National Laboratories
(Sandia National Laboratories is a multi-program laboratory managed and
operated by Sandia Corporation, a wholly owned subsidiary of Lockheed
Martin Corporation, for the U.S. Department of Energy's National Nuclear
Security Administration under contract DE-AC04-94AL85000.), Xcel Energy
through the Renewable Development Fund (grant RD4-13) and NSF Career
Award (NSF-CBET-1454259) for J.H. Computational resources were provided
by Sandia National Laboratories, National Renewable Energy Laboratory,
and the University of Minnesota Supercomputing Institute.
NR 43
TC 0
Z9 0
U1 9
U2 9
PU CAMBRIDGE UNIV PRESS
PI NEW YORK
PA 32 AVENUE OF THE AMERICAS, NEW YORK, NY 10013-2473 USA
SN 0022-1120
EI 1469-7645
J9 J FLUID MECH
JI J. Fluid Mech.
PD OCT 10
PY 2016
VL 804
BP 90
EP 115
DI 10.1017/jfm.2016.503
PG 26
WC Mechanics; Physics, Fluids & Plasmas
SC Mechanics; Physics
GA DX0WU
UT WOS:000384087900011
ER
PT J
AU Li, ZP
Liu, SG
Zhang, XS
West, TO
Ogle, SM
Zhou, NJ
AF Li, Zhengpeng
Liu, Shuguang
Zhang, Xuesong
West, Tristram O.
Ogle, Stephen M.
Zhou, Naijun
TI Evaluating land cover influences on model uncertainties-A case study of
cropland carbon dynamics in the Mid-Continent Intensive Campaign region
SO ECOLOGICAL MODELLING
LA English
DT Article
DE Biogeochemical model; Cropland carbon fluxes; Land cover; Uncertainty;
Mid-Continent Intensive Campaign
ID NET PRIMARY PRODUCTIVITY; UNITED-STATES; SPATIAL ASSOCIATION; DISTANCE
STATISTICS; TERRESTRIAL; RESOLUTION; SOIL; INVERSIONS; NPP
AB Quantifying spatial and temporal patterns of carbon sources and sinks and their uncertainties across agriculture-dominated areas remains challenging for understanding regional carbon cycles. Characteristics of local land cover inputs could impact the regional carbon estimates but the effect has not been fully evaluated in the past. Within the North American Carbon Program Mid-Continent Intensive (MCI) Campaign, three models were developed to estimate carbon fluxes on croplands: an inventory-based model, the Environmental Policy Integrated Climate (EPIC) model, and the General Ensemble biogeochemical Modeling System (GEMS) model. They all provided estimates of three major carbon fluxes on cropland: net primary production (NPP), net ecosystem production (NEP), and soil organic carbon (SOC) change. Using data mining and spatial statistics, we studied the spatial distribution of the carbon fluxes uncertainties and the relationships between the uncertainties and the land cover characteristics. Results indicated that uncertainties for all three carbon fluxes were not randomly distributed, but instead formed multiple clusters within the MCI region. We investigated the impacts of three land cover characteristics on the fluxes uncertainties: cropland percentage, cropland richness and cropland diversity. The results indicated that cropland percentage significantly influenced the uncertainties of NPP and NEP, but not on the uncertainties of SOC change. Greater uncertainties of NPP and NEP were found in counties with small cropland percentage than the counties with large cropland percentage. Cropland species richness and diversity also showed negative correlations with the model uncertainties. Our study demonstrated that the land cover characteristics contributed to the uncertainties of regional carbon fluxes estimates. The approaches we used in this study can be applied to other ecosystem models to identify the areas with high uncertainties and where models can be improved to reduce overall uncertainties for regional carbon flux estimates. (C) 2016 Elsevier B.V. All rights reserved.
C1 [Li, Zhengpeng] South Dakota State Univ, Geospatial Sci Ctr Excellence, Brookings, SD 57007 USA.
[Liu, Shuguang] US Geol Survey, Earth Resources Observat & Sci EROS Ctr, Sioux Falls, SD 57198 USA.
[Zhang, Xuesong] Pacific Northwest Natl Lab, Joint Global Change Res Inst, College Pk, MD 20740 USA.
[West, Tristram O.] US DOE, SC-23, Washington, DC 20585 USA.
[Ogle, Stephen M.] Colorado State Univ, Nat Resource Ecol Lab, Ft Collins, CO 80523 USA.
[Zhou, Naijun] Univ Maryland, Dept Geog Sci, College Pk, MD 20742 USA.
RP Li, ZP (reprint author), South Dakota State Univ, Geospatial Sci Ctr Excellence, Brookings, SD 57007 USA.
EM zli2807@jacks.sdstate.edu
RI zhang, xuesong/B-7907-2009
FU U.S. Geological Survey (USGS) Land Change Science Program; EPIC; U.S.
Department of Energy (DOE) Great Lakes Bioenergy Research Center;
National Aeronautics and Space Administration (NASA) [NNH12AU03I,
NNH13ZDA001N]; NASA Terrestrial Ecology Program [NNX08AK08G]
FX We thank Dr. Michael C. Wimberly and two anonymous reviewers for their
specific comments and helpful suggestions in improving the manuscript.
Dr. Shuguang Liu, with support from the U.S. Geological Survey (USGS)
Land Change Science Program, contributed to data analysis and writing of
the paper. The fund for EPIC modeling and Dr. Xuesong Zhang is provided
by the U.S. Department of Energy (DOE) Great Lakes Bioenergy Research
Center and the National Aeronautics and Space Administration (NASA)
(NNH12AU03I and NNH13ZDA001N). Contributions from Drs. Stephen Ogle and
Tristram West are funded by a grant from NASA Terrestrial Ecology
Program (NNX08AK08G).
NR 31
TC 0
Z9 0
U1 14
U2 18
PU ELSEVIER SCIENCE BV
PI AMSTERDAM
PA PO BOX 211, 1000 AE AMSTERDAM, NETHERLANDS
SN 0304-3800
EI 1872-7026
J9 ECOL MODEL
JI Ecol. Model.
PD OCT 10
PY 2016
VL 337
BP 176
EP 187
DI 10.1016/j.ecolmodel.2016.07.002
PG 12
WC Ecology
SC Environmental Sciences & Ecology
GA DV0EQ
UT WOS:000382591200018
ER
PT J
AU Wheatley, NM
Eden, KD
Ngo, J
Rosinski, JS
Sawaya, MR
Cascio, D
Collazo, M
Hoveida, H
Hubbell, WL
Yeates, TO
AF Wheatley, Nicole M.
Eden, Kevin D.
Ngo, Joanna
Rosinski, Justin S.
Sawaya, Michael R.
Cascio, Duilio
Collazo, Michael
Hoveida, Hamidreza
Hubbell, Wayne L.
Yeates, Todd O.
TI A PII-Like Protein Regulated by Bicarbonate: Structural and Biochemical
Studies of the Carboxysome-Associated CPII Protein
SO JOURNAL OF MOLECULAR BIOLOGY
LA English
DT Article
DE nitrogen regulatory PII proteins; bicarbonate; allostery; carbon
concentrating mechanism; carboxysome
ID SIGNAL-TRANSDUCTION PROTEIN; CARBON-CONCENTRATING MECHANISMS; PENTAMERIC
VERTEX PROTEINS; SYNECHOCYSTIS SP PCC-6803; SYNECHOCOCCUS SP PCC7002;
FACILITATE CO2 FIXATION; P-II PROTEIN; ESCHERICHIA-COLI;
CRYSTAL-STRUCTURE; INORGANIC CARBON
AB Autotrophic bacteria rely on various mechanisms to increase intracellular concentrations of inorganic forms of carbon (i.e., bicarbonate and CO2) in order to improve the efficiency with which they can be converted to organic forms. Transmembrane bicarbonate transporters and carboxysomes play key roles in accumulating bicarbonate and CO2, but other regulatory elements of carbon concentration mechanisms in bacteria are less understood. In this study, after analyzing the genomic regions around a-type carboxysome operons, we characterize a protein that is conserved across these operons but has not been previously studied. On the basis of a series of apo- and ligand-bound crystal structures and supporting biochemical data, we show that this protein, which we refer to as the carboxysome-associated PII protein (CPII), represents a new and distinct subfamily within the broad superfamily of previously studied PII regulatory proteins, which are generally involved in regulating nitrogen metabolism in bacteria. CPII undergoes dramatic conformational changes in response to ADP binding, and the affinity for nucleotide binding is strongly enhanced by the presence of bicarbonate. CPII therefore appears to be a unique type of PII protein that senses bicarbonate availability, consistent with its apparent genomic association with the carboxysome and its constituents. (C) 2016 Elsevier Ltd. All rights reserved.
C1 [Wheatley, Nicole M.; Sawaya, Michael R.; Cascio, Duilio; Collazo, Michael; Yeates, Todd O.] Univ Calif Los Angeles, DOE Inst Genom & Prote, Los Angeles, CA 90095 USA.
[Eden, Kevin D.; Ngo, Joanna; Rosinski, Justin S.; Hoveida, Hamidreza; Hubbell, Wayne L.; Yeates, Todd O.] Univ Calif Los Angeles, Dept Chem & Biochem, Los Angeles, CA 90095 USA.
[Hubbell, Wayne L.] Univ Calif Los Angeles, Jules Stein Eye Inst, Los Angeles, CA 90095 USA.
RP Yeates, TO (reprint author), Univ Calif Los Angeles, DOE Inst Genom & Prote, Los Angeles, CA 90095 USA.; Yeates, TO (reprint author), Univ Calif Los Angeles, Dept Chem & Biochem, Los Angeles, CA 90095 USA.
EM yeates@mbi.ucla.edu
OI Sawaya, Michael/0000-0003-0874-9043; Yeates, Todd/0000-0001-5709-9839
FU NIH [AI081146]; UCLA; BER program of the Department of Energy Office of
Science [DE-FC02-02ER63421]; National Institute of General Medical
Sciences from the National Institutes of Health [P41 GM103403]; NIH-DRIP
HEI [S10 RR029205]; DOE Office of Science [DE-AC02-06CH11357]
FX This work was supported by NIH grant AI081146 to T.O.Y. and by a UCLA
Whitcome Fellowship to N.M.W. The authors thank Dean Price, David
Savage, and Avi Flamholz for their helpful suggestions. The UCLA X-ray
diffraction facilities are supported by the BER program of the
Department of Energy Office of Science under award DE-FC02-02ER63421.
This work is based upon research conducted at the Northeastern
Collaborative Access Team beamlines, which are funded by the National
Institute of General Medical Sciences from the National Institutes of
Health (P41 GM103403). The Pilatus 6M detector on 24-ID-C beam line is
funded by a NIH-DRIP HEI grant (S10 RR029205). This research used the
resources of the Advanced Photon Source, a U.S. Department of Energy
(DOE) Office of Science User Facility operated for the DOE Office of
Science by Argonne National Laboratory under Contract No.
DE-AC02-06CH11357. We appreciate the expert help from the APS 24-ID-C
beamline staff, including Kanagalaghatta Rajashankar, Malcolm Capel,
Igor Kourinov, Jonathan Schuermann, and Narayanasami Sukumar.
NR 95
TC 0
Z9 0
U1 5
U2 5
PU ACADEMIC PRESS LTD- ELSEVIER SCIENCE LTD
PI LONDON
PA 24-28 OVAL RD, LONDON NW1 7DX, ENGLAND
SN 0022-2836
EI 1089-8638
J9 J MOL BIOL
JI J. Mol. Biol.
PD OCT 9
PY 2016
VL 428
IS 20
BP 4013
EP 4030
DI 10.1016/j.jmb.2016.07.015
PG 18
WC Biochemistry & Molecular Biology
SC Biochemistry & Molecular Biology
GA DY7QJ
UT WOS:000385324000011
PM 27464895
ER
PT J
AU Langan, PS
Close, DW
Coates, L
Rocha, RC
Ghosh, K
Kiss, C
Waldo, G
Freyer, J
Kovalevsky, A
Bradbury, ARM
AF Langan, P. S.
Close, D. W.
Coates, L.
Rocha, R. C.
Ghosh, K.
Kiss, C.
Waldo, G.
Freyer, J.
Kovalevsky, A.
Bradbury, A. R. M.
TI Evolution and Characterization of a New Reversibly Photoswitching
Chromogenic Protein, Dathail (vol 428, pg 1776, 2016)
SO JOURNAL OF MOLECULAR BIOLOGY
LA English
DT Correction
C1 [Langan, P. S.; Close, D. W.; Kiss, C.; Waldo, G.; Bradbury, A. R. M.] Los Alamos Natl Lab, Biosci Div, Los Alamos, NM 87545 USA.
[Close, D. W.; Rocha, R. C.; Ghosh, K.] Los Alamos Natl Lab, Ctr Integrated Nanotechnol, Los Alamos, NM 87545 USA.
[Close, D. W.] ARUP Labs Inst Clin & Expt Pathol, Salt Lake City, UT 84108 USA.
[Coates, L.; Kovalevsky, A.] Oak Ridge Natl Lab, Biol & Soft Matter Div, Oak Ridge, TN 37831 USA.
[Freyer, J.] Univ New Mexico, Ctr Biomed Engn, Albuquerque, NM 87131 USA.
[Langan, P. S.] Univ New Mexico, Nanosci & Microsyst Engn, Albuquerque, NM 87131 USA.
RP Bradbury, ARM (reprint author), Los Alamos Natl Lab, Div B, TA43,HRL-1,MS M888, Los Alamos, NM 87545 USA.
EM amb@LANL.gov
NR 1
TC 0
Z9 0
U1 0
U2 0
PU ACADEMIC PRESS LTD- ELSEVIER SCIENCE LTD
PI LONDON
PA 24-28 OVAL RD, LONDON NW1 7DX, ENGLAND
SN 0022-2836
EI 1089-8638
J9 J MOL BIOL
JI J. Mol. Biol.
PD OCT 9
PY 2016
VL 428
IS 20
BP 4244
EP 4244
DI 10.1016/j.jmb.2016.08.024
PG 1
WC Biochemistry & Molecular Biology
SC Biochemistry & Molecular Biology
GA DY7QJ
UT WOS:000385324000029
PM 27629583
ER
PT J
AU Kassebaum, NJ
Arora, M
Barber, RM
Bhutta, ZA
Carter, A
Casey, DC
Charlson, FJ
Coates, MM
Coggeshall, M
Cornaby, L
Dandona, L
Dicker, DJ
Erskine, HE
Ferrari, AJ
Fitzmaurice, C
Foreman, K
Forouzanfar, MH
Fullman, N
Gething, PW
Goldberg, EM
Graetz, N
Haagsma, JA
Johnson, C
Kemmer, L
Khalil, IA
Kinfu, Y
Kutz, MJ
Kyu, HH
Leung, J
Liang, XF
Lim, SS
Lim, SS
Lozano, R
Mensah, GA
Mikesell, J
Mokdad, AH
Mooney, MD
Naghavi, M
Nguyen, G
Nsoesie, E
Pigott, DM
Pinho, C
Rankin, Z
Reinig, N
Salomon, JA
Sandar, L
Smith, A
Sorensen, RJD
Stanaway, J
Steiner, C
Teeple, S
Thomas, BA
Troeger, C
VanderZanden, A
Wagner, JA
Wanga, V
Whiteford, HA
Zhou, M
Zoeckler, L
Abajobir, AA
Abate, KH
Abbafati, C
Abbas, KM
Abd-Allah, F
Abraham, B
Abubakar, I
Abu-Raddad, LJ
Abu-Rmeileh, NME
Achoki, T
Ackerman, IN
Adebiyi, AO
Adedeji, IA
Adsuar, JC
Afanvi, KA
Afshin, A
Agardh, EE
Agarwal, A
Kumar, S
Ahmed, MB
Kiadaliri, AA
Ahmadieh, H
Akseer, N
Al-Aly, Z
Alam, K
Alam, NKM
Aldhahri, SF
Alegretti, MA
Aleman, AV
Alemu, ZA
Alexander, LT
Raghib, A
Alkerwi, A
Alla, F
Allebeck, P
Alsharif, U
Altirkawi, KA
Martin, EA
Alvis-Guzman, N
Amare, AT
Amberbir, A
Amegah, AK
Amini, H
Ammar, W
Amrock, SM
Anderson, GM
Anderson, BO
Antonio, CAT
Anwari, P
Arnlov, J
Arsenijevic, VSA
Artaman, A
Asayesh, H
Asghar, RJ
Avokpaho, EFGA
Awasthi, A
Quintanilla, BPA
Azzopardi, P
Bacha, U
Badawi, A
Balakrishnan, K
Banerjee, A
Barac, A
Barker-Collo, SL
Barnighausen, T
Barregard, L
Barrero, LH
Basu, S
Bayou, TA
Beardsley, J
Bedi, N
Beghi, E
Bell, B
Bell, ML
Benjet, C
Bennett, DA
Bensenor, IM
Berhane, A
Bernabe, E
Betsu, BD
Beyene, AS
Bhala, N
Bhansali, A
Bhatt, S
Biadgilign, S
Bienhofff, K
Bikbov, B
Bin Abdulhak, AA
Bisanzio, D
Bjertness, E
Blore, JD
Borschmann, R
Boufous, S
Bourne, RRA
Brainin, M
Brazinova, A
Breitborde, NJK
Brugha, TS
Buchbinder, R
Buckle, GC
Butt, ZA
Calabria, B
Campos-Nonato, IR
Campuzano, JC
Carabin, H
Carapetis, JR
Cardenas, R
Carrero, JJ
Castaneda-Orjuela, CA
Rivas, JC
Catala-Lopez, F
Cavalleri, F
Chang, JC
Chiang, PPC
Chibalabala, M
Chibueze, CE
Chisumpa, VH
Choi, JYJ
Choudhury, L
Christensen, H
Ciobanu, LG
Colistro, V
Colomar, M
Colquhoun, SM
Cortinovis, M
Crump, JA
Damasceno, A
Dandona, R
Dargan, PI
Das Neves, J
Davey, G
Davis, AC
De Leo, D
Degenhardt, L
Del Gobbo, LC
Derrett, S
Des Jarlais, DC
Deveber, GA
Dharmaratne, SD
Dhillon, PK
Ding, EL
Doyle, KE
Driscoll, TR
Duan, L
Dubey, M
Duncan, BB
Ebrahimi, H
Ellenbogen, RG
Elyazar, I
Endries, AY
Ermakov, SP
Eshrati, B
Esteghamati, A
Estep, K
Fahimi, S
Farid, TA
Farinha, CSES
Faro, A
Farvid, MS
Farzadfar, F
Feigin, VL
Fereshtehnejad, SM
Fernandes, JG
Fernandes, JC
Fischer, F
Fitchett, JRA
Foigt, N
Fowkes, FGR
Franklin, RC
Friedman, J
Frostad, J
Furst, T
Futran, ND
Gabbe, B
Gankpe, FG
Garcia-Basteiro, AL
Gebrehiwot, TT
Gebremedhin, AT
Geleijnse, JM
Gibney, KB
Gillum, RF
Ginawi, IAM
Giref, AZ
Giroud, M
Gishu, MD
Godwin, WW
Gomez-Dantes, H
Gona, P
Goodridge, A
Gopalani, SV
Gotay, CC
Goto, A
Gouda, HN
Guo, Y
Gupta, R
Gupta, R
Gupta, V
Gutierrez, RA
Hafezi-Nejad, N
Haile, D
Hailu, AD
Hailu, GB
Halasa, YA
Ribhi, R
Hamadeh
Hamidi, S
Hammami, M
Handal, AJ
Hankey, GJ
Harb, HL
Harikrishnan, S
Haro, JM
Hassanvand, MS
Hassen, TA
Havmoeller, R
Hay, RJ
Hedayati, MT
Heredia-Pi, IB
Heydarpour, P
Hoek, HW
Hoffman, DJ
Horino, M
Horita, N
Hosgood, HD
Hoy, DG
Hsairi, M
Huang, H
Huang, JJ
Iburg, KM
Idrisov, BT
Innos, K
Inoue, M
Jacobsen, KH
Jauregui, A
Jayatilleke, AU
Jeemon, P
Jha, V
Jiang, GH
Jiang, Y
Jibat, T
Jimenez-Corona, A
Jin, Y
Jonas, JB
Kabir, Z
Kajungu, DK
Kalkonde, Y
Kamal, R
Kan, HD
Kandel, A
Karch, A
Karema, CK
Karimkhani, C
Kasaeian, A
Katibeh, M
Kaul, A
Kawakami, N
Kazi, DS
Keiyoro, PN
Kemp, AH
Kengne, AP
Keren, A
Kesavachandran, CN
Khader, YS
Khan, AR
Khan, EA
Khang, YH
Khoja, TAM
Khubchandani, J
Kieling, C
Kim, CI
Kim, D
Kim, YJ
Kissoon, N
Kivipelto, M
Knibbs, LD
Knudsen, AK
Kokubo, Y
Kolte, D
Kopec, JA
Koul, PA
Koyanagi, A
Defo, BK
Kuchenbecker, RS
Bicer, BK
Kuipers, EJ
Kumar, GA
Kwan, GF
Lalloo, R
Lallukka, T
Larsson, A
Latif, AA
Lavados, PM
Lawrynowicz, AEB
Leasher, JL
Leigh, J
Leung, R
Li, YC
Li, YM
Lipshultz, SE
Liu, PY
Liu, Y
Lloyd, BK
Logroscino, G
Looker, KJ
Lotufo, PA
Lucas, RM
Lunevicius, R
Lyons, RA
El Razek, HMA
Mandavi, M
Majdan, M
Majeed, A
Malekzadeh, R
Malta, DC
Marcenes, W
Martinez-Raga, J
Masiye, F
Mason-Jones, AJ
Matzopoulos, R
Mayosi, BM
McGrath, JJ
Mckee, M
Meaney, PA
Mehari, A
Melaku, YA
Memiah, P
Memish, ZA
Mendoza, W
Meretoja, A
Meretoja, TJ
Mesfin, YM
Mhimbira, FA
Miller, TR
Mills, EJ
Mirarefin, M
Mirrakhimov, EM
Mitchell, PB
Mock, CN
Mohammad, KA
Mohammadi, A
Mohammed, S
Monasta, L
Hernandez, JCM
Montico, M
Moradi-Lakeh, M
Mori, R
Mueller, UO
Mumford, JE
Murdoch, ME
Murthy, GVS
Nachega, JB
Naheed, A
Naldi, L
Nangia, V
Newton, JN
Ng, M
Ngalesoni, FN
Le Nguyen, Q
Nisar, MI
Pete, PMN
Nolla, JM
Norheim, OF
Norman, RE
Norrving, B
Obermeyer, CM
Ogbo, FA
Oh, IH
Oladimeji, O
Olivares, PR
Olusanya, BO
Olusanya, JO
Oren, E
Ortiz, A
Ota, E
Oyekale, AS
Pa, M
Park, EK
Parsaeian, M
Patten, SB
Patton, GC
Pedro, JM
Pereira, DM
Perico, N
Pesudovs, K
Petzold, M
Phillips, MR
Piel, FB
Pillay, JD
Pishgar, F
Plass, D
Polinder, S
Popova, S
Poulton, RG
Pourmalek, F
Prasad, NM
Qorbani, M
Rabiee, RHS
Radfar, A
Rafay, A
Rahimi, K
Rahimi-Movaghar, V
Rahman, M
Rahman, MHU
Rahman, SU
Rai, D
Rai, RK
Rajsic, S
Raju, M
Ram, U
Ranganathan, K
Refaat, AH
Reitsma, MB
Remuzzi, G
Resnikoff, S
Reynolds, A
Ribeiro, AL
Ricci, S
Roba, HS
Rojas-Rueda, D
Ronfani, L
Roshandel, G
Roth, GA
Roy, A
Sackey, BB
Sagar, R
Sanabria, JR
Sanchez-Nino, MD
Santos, IS
Santos, JV
Sarmiento-Suarez, R
Sartorius, B
Satpathy, M
Savic, M
Sawhney, M
Schmidt, MI
Schneider, IJC
Schutte, AE
Schwebel, DC
Seedat, S
Sepanlou, SG
Servan-Mori, EE
Shahraz, S
Shaikh, MA
Sharma, R
She, J
Sheikhbahaei, S
Shen, J
Sheth, KN
Shibuya, K
Shigematsu, M
Shin, MJ
Shin, R
Sigfusdottir, ID
Silva, DAS
Silverberg, JI
Simard, EP
Singh, A
Singh, JA
Singh, PK
Skirbekk, V
Skogen, JC
Soljak, M
Soreide, K
Sorensen, RJD
Sreeramareddy, CT
Stathopoulou, V
Steel, N
Stein, DJ
Stein, MB
Steiner, TJ
Stovner, LJ
Stranges, S
Stroumpoulis, K
Sunguya, BF
Sur, PJ
Swaminathan, S
Sykes, BL
Szoeke, CEI
Tabares-Seisdedos, R
Landon, N
Tanne, D
Tavakkoli, M
Taye, B
Taylor, HR
Ao, BJT
Tegegne, TK
Tekle, DY
Terkawi, AS
Tessema, GA
Thakur, JS
Thomson, AJ
Thorne-Lyman, AL
Thrift, AG
Thurston, GD
Tobe-Gai, R
Tonelli, M
Topor-Madry, R
Topouzis, F
Tran, BX
Dimbuene, ZT
Tsilimbaris, M
Tura, AK
Tuzcu, EM
Tyrovolas, S
Ukwaja, KN
Undurraga, EA
Uneke, CJ
Uthman, OA
van Gool, CH
van Os, J
Vasankari, T
Vasconcelos, AMN
Venketasubramanian, N
Violante, FS
Vlassov, VV
Vollset, SE
Wagner, GR
Wallin, MT
Wang, LH
Weichenthal, S
Weiderpass, E
Weintraub, RG
Werdecker, A
WestermaM, R
Wijeratne, T
Wilkinson, JD
Williams, HC
Wiysonge, CS
Woldeyohannes, SM
Wolfe, CDA
Won, S
Xu, G
Yadav, AK
Yakob, B
Yan, LL
Yan, Y
Yaseri, M
Ye, P
Yip, P
Yonemoto, N
Yoon, SJ
Younis, MZ
Yu, C
Zaidi, Z
Zaki, MES
Zeeb, H
Zodpey, S
Zonies, D
Zuhlke, LJ
Zeeb, H
Zodpey, S
Zonies, D
Zuhlke, LJ
Vos, T
Lopez, AD
Murray, CJL
AF Kassebaum, Nicholas J.
Arora, Megha
Barber, Ryan M.
Bhutta, Zulfigar A.
Carter, Austin
Casey, Daniel C.
Charlson, Fiona J.
Coates, Matthew M.
Coggeshall, Megan
Cornaby, Leslie
Dandona, Lalit
Dicker, Daniel J.
Erskine, Holly E.
Ferrari, Alize J.
Fitzmaurice, Christina
Foreman, Kyle
Forouzanfar, Mohammad H.
Fullman, Nancy
Gething, Peter W.
Goldberg, Ellen M.
Graetz, Nicholas
Haagsma, Juanita A.
Johnson, Catherine
Kemmer, Laura
Khalil, Ibrahim A.
Kinfu, Yohannes
Kutz, Michael J.
Kyu, Hmwe H.
Leung, Janni
Liang, Xiaofeng
Lim, Stephen S.
Lim, Stephen S.
Lozano, Rafael
Mensah, George A.
Mikesell, Joe
Mokdad, Ali H.
Mooney, Meghan D.
Naghavi, Mohsen
Nguyen, Grant
Nsoesie, Elaine
Pigott, David M.
Pinho, Christine
Rankin, Zane
Reinig, Nikolas
Salomon, Joshua A.
Sandar, Logan
Smith, Alison
Sorensen, Reed J. D.
Stanaway, Jeffrey
Steiner, Caitlyn
Teeple, Stephanie
Thomas, Bernadette A.
Troeger, Chris
VanderZanden, Amelia
Wagner, Joseph A.
Wanga, Valentine
Whiteford, Harvey A.
Zhou, Maigeng
Zoeckler, Leo
Abajobir, Amanuel Alemu
Abate, Kalkidan Hassen
Abbafati, Cristiana
Abbas, Kaja M.
Abd-Allah, Foad
Abraham, Biju
Abubakar, Ibrahim
Abu-Raddad, Laith J.
Abu-Rmeileh, Niveen M. E.
Achoki, Tom
Ackerman, Ilana N.
Adebiyi, Akindele Olupelumi
Adedeji, Isaac Akinkunmi
Adsuar, Jose C.
Afanvi, Kossivi Agbelenko
Afshin, Ashkan
Agardh, Emilie Elisabet
Agarwal, Arnav
Kumar, Sanjay
Ahmed, Muktar Beshir
Kiadaliri, Aliasghar Ahmad
Ahmadieh, Hamid
Akseer, Nadia
Al-Aly, Ziyad
Alam, Khurshid
Alam, Noore K. M.
Aldhahri, Saleh Fahed
Alegretti, Miguel Angel
Aleman, Alicia V.
Alemu, Zewdie Aderaw
Alexander, Lily T.
Raghib, Ali
Alkerwi, Ala'a
Alla, Francois
Allebeck, Peter
Alsharif, Ubai
Altirkawi, Khalid A.
Martin, Elena Alvarez
Alvis-Guzman, Nelson
Amare, Azmeraw T.
Amberbir, Alemayehu
Amegah, Adeladza Kofi
Amini, Heresh
Ammar, Walid
Amrock, Stephen Marc
Anderson, Gregory M.
Anderson, Benjamin O.
Antonio, Carl Abelardo T.
Anwari, Palwasha
Arnlov, Johan
Arsenijevic, Valentina S. Arsic
Artaman, Al
Asayesh, Hamid
Asghar, Rana Jawad
Avokpaho, Euripide Frinel G. Arthur
Awasthi, Ashish
Quintanilla, Beatriz Paulina Ayala
Azzopardi, Peter
Bacha, Umar
Badawi, Alaa
Balakrishnan, Kalpana
Banerjee, Amitava
Barac, Aleksandra
Barker-Collo, Suzanne L.
Barnighausen, Till
Barregard, Lars
Barrero, Lope H.
Basu, Sanjay
Bayou, Tigist Assefa
Beardsley, Justin
Bedi, Neeraj
Beghi, Ettore
Bell, Brent
Bell, Michelle L.
Benjet, Corina
Bennett, Derrick A.
Bensenor, Isabela M.
Berhane, Adugnaw
Bernabe, Eduardo
Betsu, Balem Demtsu
Beyene, Addisu Shunu
Bhala, Neeraj
Bhansali, Anil
Bhatt, Samir
Biadgilign, Sibhatu
Bienhofff, Kelly
Bikbov, Boris
Bin Abdulhak, Aref A.
Bisanzio, Donal
Bjertness, Espen
Blore, Jed D.
Borschmann, Rohan
Boufous, Soufiane
Bourne, Rupert R. A.
Brainin, Michael
Brazinova, Alexandra
Breitborde, Nicholas J. K.
Brugha, Traolach S.
Buchbinder, Rachelle
Buckle, Geoffrey Colin
Butt, Zahid A.
Calabria, Bianca
Campos-Nonato, Ismael Ricardo
Campuzano, Julio Cesar
Carabin, Helene
Carapetis, Jonathan R.
Cardenas, Rosario
Carrero, Juan Jesus
Castaneda-Orjuela, Carlos A.
Rivas, Jacqueline Castillo
Catala-Lopez, Ferran
Cavalleri, Fiorella
Chang, Jung-Chen
Chiang, Peggy Pei-Chia
Chibalabala, Mirriam
Chibueze, Chioma Ezinne
Chisumpa, Vesper Hichilombwe
Choi, Jee-Young Jasmine
Choudhury, Lincoln
Christensen, Hanne
Ciobanu, Liliana G.
Colistro, Valentina
Colomar, Mercedes
Colquhoun, Samantha M.
Cortinovis, Monica
Crump, John A.
Damasceno, Albertino
Dandona, Rakhi
Dargan, Paul I.
Das Neves, Jose
Davey, Gail
Davis, Adrian C.
De Leo, Diego
Degenhardt, Louisa
Del Gobbo, Liana C.
Derrett, Sarah
Des Jarlais, Don C.
Deveber, Gabrielle A.
Dharmaratne, Samath D.
Dhillon, Preet K.
Ding, Eric L.
Doyle, Kerrie E.
Driscoll, Tim R.
Duan, Leilei
Dubey, Manisha
Duncan, Bruce Bartholow
Ebrahimi, Hedyeh
Ellenbogen, Richard G.
Elyazar, Iqbal
Endries, Aman Yesuf
Ermakov, Sergey Petrovich
Eshrati, Babak
Esteghamati, Alireza
Estep, Kara
Fahimi, Saman
Farid, Talha A.
Sa Farinha, Carla Sofia e
Faro, Andre
Farvid, Maryam S.
Farzadfar, Farshad
Feigin, Valery L.
Fereshtehnejad, Seyed-Mohammad
Fernandes, Jefferson G.
Fernandes, Joao C.
Fischer, Florian
Fitchett, Joseph R. A.
Foigt, Nataliya
Fowkes, F. Gerry R.
Franklin, Richard C.
Friedman, Joseph
Frostad, Joseph
Furst, Thomas
Futran, Neal D.
Gabbe, Belinda
Gankpe, Fortune Gbetoho
Garcia-Basteiro, Alberto L.
Gebrehiwot, Tsegaye Tewelde
Gebremedhin, Amanuel Tesfay
Geleijnse, Johanna M.
Gibney, Katherine B.
Gillum, Richard F.
Ginawi, Ibrahim Abdelmageem Mohamed
Giref, Ababi Zergaw
Giroud, Maurice
Gishu, Melkamu Dedefo
Godwin, William W.
Gomez-Dantes, Hector
Gona, Philimon
Goodridge, Amador
Gopalani, Sameer Vali
Gotay, Carolyn C.
Goto, Atsushi
Gouda, Hebe N.
Guo, Yuming
Gupta, Rahul
Gupta, Rajeev
Gupta, Vipin
Gutierrez, Reyna A.
Hafezi-Nejad, Nima
Haile, Demewoz
Hailu, Alemayehu Desalegne
Hailu, Gessessew Bugssa
Halasa, Yara A.
Ribhi, Randah
Hamadeh
Hamidi, Samer
Hammami, Mouhanad
Handal, Alexis J.
Hankey, Graeme J.
Harb, Hilda L.
Harikrishnan, Sivadasanpillai
Haro, Josep Maria
Hassanvand, Mohammad Sadegh
Hassen, Tahir Ahmed
Havmoeller, Rasmus
Hay, Roderick J.
Hedayati, Mohammad T.
Heredia-Pi, Ileana Beatriz
Heydarpour, Pouria
Hoek, Hans W.
Hoffman, Daniel J.
Horino, Masako
Horita, Nobuyuki
Hosgood, H. Dean
Hoy, Damian G.
Hsairi, Mohamed
Huang, Hsiang
Huang, John J.
Iburg, Kim Moesgaard
Idrisov, Bulat T.
Innos, Kaire
Inoue, Manami
Jacobsen, Kathryn H.
Jauregui, Alejandra
Jayatilleke, Achala Upendra
Jeemon, Panniyammakal
Jha, Vivekanand
Jiang, Guohong
Jiang, Ying
Jibat, Tariku
Jimenez-Corona, Aida
Jin, Ye
Jonas, Jost B.
Kabir, Zubair
Kajungu, Dan K.
Kalkonde, Yogeshwar
Kamal, Ritul
Kan, Haidong
Kandel, Amit
Karch, Andre
Karema, Corine Kakizi
Karimkhani, Chante
Kasaeian, Amir
Katibeh, Marzieh
Kaul, Anil
Kawakami, Norito
Kazi, Dhruv S.
Keiyoro, Peter Njenga
Kemp, Andrew Haddon
Kengne, Andre Pascal
Keren, Andre
Kesavachandran, Chandrasekharan Nair
Khader, Yousef Saleh
Khan, Abdur Rahman
Khan, Ejaz Ahmad
Khang, Young-Ho
Khoja, Tawfik Ahmed Muthafer
Khubchandani, Jagdish
Kieling, Christian
Kim, Cho-il
Kim, Daniel
Kim, Yun Jin
Kissoon, Niranjan
Kivipelto, Miia
Knibbs, Luke D.
Knudsen, Ann Kristin
Kokubo, Yoshihiro
Kolte, Dhaval
Kopec, Jacek A.
Koul, Parvaiz A.
Koyanagi, Ai
Defo, Barthelemy Kuate
Kuchenbecker, Ricardo S.
Bicer, Burcu Kucuk
Kuipers, Ernst J.
Kumar, G. Anil
Kwan, Gene F.
Lalloo, Ratilal
Lallukka, Tea
Larsson, Anders
Latif, Asma Abdul
Lavados, Pablo M.
Lawrynowicz, Alicia Elena Beatriz
Leasher, Janet L.
Leigh, James
Leung, Ricky
Li, Yichong
Li, Yongmei
Lipshultz, Steven E.
Liu, Patrick Y.
Liu, Yang
Lloyd, Belinda K.
Logroscino, Giancarlo
Looker, Katharine J.
Lotufo, Paulo A.
Lucas, Robyn M.
Lunevicius, Raimundas
Lyons, Ronan A.
El Razek, Hassan Magdy Abd
Mandavi, Mandi
Majdan, Marek
Majeed, Azeem
Malekzadeh, Reza
Malta, Deborah Carvalho
Marcenes, Wagner
Martinez-Raga, Jose
Masiye, Felix
Mason-Jones, Amanda J.
Matzopoulos, Richard
Mayosi, Bongani M.
McGrath, John J.
Mckee, Martin
Meaney, Peter A.
Mehari, Alem
Melaku, Yohannes Adama
Memiah, Peter
Memish, Ziad A.
Mendoza, Walter
Meretoja, Atte
Meretoja, Tuomo J.
Mesfin, Yonatan Moges
Mhimbira, Francis Apolinary
Miller, Ted R.
Mills, Edward J.
Mirarefin, Mojde
Mirrakhimov, Erkin M.
Mitchell, Philip B.
Mock, Charles N.
Mohammad, Karzan Abdulmuhsin
Mohammadi, Alireza
Mohammed, Shafiu
Monasta, Lorenzo
Montanez Hernandez, Julio Cesar
Montico, Marcella
Moradi-Lakeh, Maziar
Mori, Rintaro
Mueller, Ulrich O.
Mumford, John Everett
Murdoch, Michele E.
Murthy, Gudlavalleti Venkata Satyanarayana
Nachega, Jean B.
Naheed, Aliya
Naldi, Luigi
Nangia, Vinay
Newton, John N.
Ng, Marie
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CA GBD 2015 DALY & HALE
TI Global, regional, and national disability-adjusted life-years (DALYs)
for 315 diseases and injuries and healthy life expectancy (HALE),
1990-2015: a systematic analysis for the Global Burden of Disease Study
2015
SO LANCET
LA English
DT Article
ID SUSTAINABLE DEVELOPMENT GOALS; UNITED-STATES; 187 COUNTRIES; BACK-PAIN;
COMPRESSION; TRENDS; RECOMMENDATIONS; PREVALENCE; MORBIDITY; MORTALITY
AB Background Healthy life expectancy (HALE) and disability-adjusted life-years (DALYs) provide summary measures of health across geographies and time that can inform assessments of epidemiological patterns and health system performance, help to prioritise investments in research and development, and monitor progress toward the Sustainable Development Goals (SDGs). We aimed to provide updated HALE and DALYs for geographies worldwide and evaluate how disease burden changes with development.
Methods We used results from the Global Burden of Diseases, Injuries, and Risk Factors Study 2015 (GBD 2015) for all-cause mortality, cause-specific mortality, and non-fatal disease burden to derive HALE and DALYs by sex for 195 countries and territories from 1990 to 2015. We calculated DALYs by summing years of life lost (YLLs) and years of life lived with disability (YLDs) for each geography, age group, sex, and year. We estimated HALE using the Sullivan method, which draws from age-specific death rates and YLDs per capita. We then assessed how observed levels of DALYs and HALE differed from expected trends calculated with the Socio-demographic Index (SDI), a composite indicator constructed from measures of income per capita, average years of schooling, and total fertility rate.
Findings Total global DALYs remained largely unchanged from 1990 to 2015, with decreases in communicable, neonatal, maternal, and nutritional (Group 1) disease DALYs off set by increased DALYs due to non-communicable diseases (NCDs). Much of this epidemiological transition was caused by changes in population growth and ageing, but it was accelerated by widespread improvements in SDI that also correlated strongly with the increasing importance of NCDs. Both total DALYs and age-standardised DALY rates due to most Group 1 causes significantly decreased by 2015, and although total burden climbed for the majority of NCDs, age-standardised DALY rates due to NCDs declined. Nonetheless, age-standardised DALY rates due to several high-burden NCDs (including osteoarthritis, drug use disorders, depression, diabetes, congenital birth defects, and skin, oral, and sense organ diseases) either increased or remained unchanged, leading to increases in their relative ranking in many geographies. From 2005 to 2015, HALE at birth increased by an average of 2.9 years (95% uncertainty interval 2.9-3.0) for men and 3.5 years (3.4-3.7) for women, while HALE at age 65 years improved by 0.85 years (0.78-0.92) and 1.2 years (1.1-1.3), respectively. Rising SDI was associated with consistently higher HALE and a somewhat smaller proportion of life spent with functional health loss; however, rising SDI was related to increases in total disability. Many countries and territories in central America and eastern sub-Saharan Africa had increasingly lower rates of disease burden than expected given their SDI. At the same time, a subset of geographies recorded a growing gap between observed and expected levels of DALYs, a trend driven mainly by rising burden due to war, interpersonal violence, and various NCDs.
Interpretation Health is improving globally, but this means more populations are spending more time with functional health loss, an absolute expansion of morbidity. The proportion of life spent in ill health decreases somewhat with increasing SDI, a relative compression of morbidity, which supports continued efforts to elevate personal income, improve education, and limit fertility. Our analysis of DALYs and HALE and their relationship to SDI represents a robust framework on which to benchmark geography-specific health performance and SDG progress. Country-specific drivers of disease burden, particularly for causes with higher-than-expected DALYs, should inform financial and research investments, prevention efforts, health policies, and health system improvement initiatives for all countries along the development continuum. Copyright (C) The Author(s). Published by Elsevier Ltd.
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[Calabria, Bianca; Mitchell, Philip B.] Univ New S Wales, Kensington, NSW, Australia.
[Campos-Nonato, Ismael Ricardo; Campuzano, Julio Cesar; Gomez-Dantes, Hector; Heredia-Pi, Ileana Beatriz; Jauregui, Alejandra; Montanez Hernandez, Julio Cesar; Servan-Mori, Edson E.] Natl Inst Publ Hlth, Cuernavaca, Morelos, Mexico.
[Carabin, Helene] Univ Oklahoma Hlth Sci Ctr, Dept Biostat & Epidemiol, Oklahoma City, OK USA.
[Carapetis, Jonathan R.] Univ Western Australia, Telethon Kids Inst, Princess Margaret Hosp Children, Subiaco, WA, Australia.
[Cardenas, Rosario] Metropolitan Autonomous Univ, Mexico City, DF, Mexico.
[Castaneda-Orjuela, Carlos A.] Colombian Natl Hlth Observ, Inst Nacl Salud, Bogota, Colombia.
[Castaneda-Orjuela, Carlos A.] Univ Nacl Colombia, Epidemiol & Publ Hlth Evaluat Grp, Dept Publ Hlth, Bogota, Colombia.
[Rivas, Jacqueline Castillo] Caja Costarricense Seguro Social, San Jose, Costa Rica.
[Rivas, Jacqueline Castillo] Univ Costa Rica, San Pedro, Montes De Oca, Costa Rica.
[Catala-Lopez, Ferran; Tabares-Seisdedos, Rafael] Univ Valencia, Dept Med, INCLIVA Hlth Res Inst & CIBERSAM, Valencia, Spain.
[Catala-Lopez, Ferran] Ottawa Hosp Res Inst, Clin Epidemiol Program, Ottawa, ON, Canada.
[Chang, Jung-Chen] Natl Taiwan Univ, Sch Nursing, Coll Med, Taipei, Taiwan.
[Chiang, Peggy Pei-Chia] Clin Governance Unit, Gold Coast Hlth, Southport, Qld, Australia.
[Chibalabala, Mirriam] Crowd Watch Afr, Lusaka, Zambia.
[Chibueze, Chioma Ezinne; Mori, Rintaro] Natl Ctr Child Hlth & Dev, Tokyo, Japan.
[Chisumpa, Vesper Hichilombwe; Masiye, Felix] Univ Zambia, Lusaka, Zambia.
[Chisumpa, Vesper Hichilombwe] Univ Witwatersrand, Johannesburg, South Africa.
[Choi, Jee-Young Jasmine] Seoul Natl Univ Med Lib, Seoul, South Korea.
[Choudhury, Lincoln] World Bank, New Delhi, India.
[Christensen, Hanne] Bispebjerg Hosp, Copenhagen, Denmark.
[Colistro, Valentina] Ministerio Salud Publ, Montevideo, Uruguay.
[Colomar, Mercedes] UNICEM, Montevideo, Uruguay.
[Crump, John A.] Univ Otago, Ctr Int Hlth, Dunedin Sch Med, Dunedin, New Zealand.
[Derrett, Sarah] Univ Otago, Injury Prevent Res Unit, Dept Prevent & Social Med, Dunedin Sch Med, Dunedin, New Zealand.
[Poulton, Richie G.] Univ Otago, Dunedin, New Zealand.
[Damasceno, Albertino] Eduardo Mondlane Univ, Fac Med, Maputo, Mozambique.
[Dargan, Paul I.] Guys & St Thomas NHS Fdn Trust, London, England.
[Das Neves, Jose] Univ Porto, Inst Invest Inovacao Sande I3S, Oporto, Portugal.
[Das Neves, Jose] Univ Porto, INEB Inst Engn Biomed, Oporto, Portugal.
[Pedro, Joao Mario] Univ Porto, EPI Unit Inst Publ Hlth, Oporto, Portugal.
[Santos, Joao Vasco] Univ Porto, Oporto, Portugal.
[Davey, Gail] Wellcome Trust Brighton Sussex Ctr Global Hlth Re, Brighton, E Sussex, England.
[Davis, Adrian C.; Newton, John N.; Steel, Nicholas] Publ Hlth England, London, England.
[De Leo, Diego] Griffith Univ, Brisbane, Qld, Australia.
[Des Jarlais, Don C.] Mt Sinai Beth Israel, New York, NY USA.
[Des Jarlais, Don C.] Icahn Sch Med Mt Sinai, New York, NY USA.
[Dharmaratne, Samath D.] Univ Peradeniya, Dept Community Med, Fac Med, Peradeniya, Sri Lanka.
[Jeemon, Panniyammakal] Ctr Control Chron Condit, Gurgaon, India.
[Dhillon, Preet K.; Zodpey, Sanjay] Publ Hlth Fdn India, Gurgaon, India.
[Doyle, Kerrie E.] RMIT Univ, Bundoora, Vic, Australia.
[Dubey, Manisha; Rahman, Mahfuzar; Ram, Usha; Singh, Abhishek; Yadav, Ajit Kumar] Int Inst Populat Sci, Mumbai, Maharashtra, India.
[Duncan, Bruce Bartholow; Kieling, Christian; Schmidt, Maria Ines] Univ Fed Rio Grande do Sul, Porto Alegre, RS, Brazil.
[Duncan, Bruce Bartholow] Univ N Carolina, Chapel Hill, NC USA.
[Ebrahimi, Hedyeh; Esteghamati, Alireza; Farzadfar, Farshad; Hafezi-Nejad, Nima; Kasaeian, Amir; Parsaeian, Mahboubeh; Pishgar, Farhad; Sheikhbahaei, Sara] Endocrinol & Metab Populat Sci Inst, Non Communicable Dis Res Ctr, Tehran, Iran.
[Ebrahimi, Hedyeh] Shariati Hosp, Digest Dis Res Inst, Liver & Pancreaticobiliary Dis Res Ctr, Tehran, Iran.
[Fahimi, Saman; Malekzadeh, Reza; Roshandel, Gholamreza; Sepanlou, Sadaf G.] Digest Dis Res Inst, Tehran, Iran.
[Hassanvand, Mohammad Sadegh] Inst Environm Res, Ctr Air Pollut Res, Tehran, Iran.
[Heydarpour, Pouria] Multiple Sclerosis Res Ctr Neurosci Inst, Tehran, Iran.
[Kasaeian, Amir] Hematol Oncol & Stem Cell Transplantat Res Ctr, Tehran, Iran.
[Parsaeian, Mahboubeh] Sch Publ Hlth, Dept Epidemiol & Biostat, Tehran, Iran.
[Pishgar, Farhad] Urooncol Res Ctr, Tehran, Iran.
[Rahimi-Movaghar, Vafa] Sina Trauma & Surg Res Ctr, Tehran, Iran.
[Yaseri, Mehdi] Univ Tehran Med Sci, Tehran, Iran.
[Elyazar, Iqbal] Eijkman Oxford Clin Res Unit, Jakarta, Indonesia.
[Endries, Aman Yesuf] Arba Minch Univ, Arba Minch, Ethiopia.
[Ermakov, Sergey Petrovich] Russian Acad Sci, Inst Social & Econ Studies Populat, Moscow, Russia.
[Ermakov, Sergey Petrovich] Russian Federat, Fed Res Inst Hlth Org & Informat, Minist Hlth, Moscow, Russia.
[Eshrati, Babak] Minist Hlth & Med Educ, Tehran, Iran.
[Eshrati, Babak] Arak Univ Med Sci, Arak, Iran.
[Farid, Talha A.; Khan, Abdur Rahman] Univ Louisville, Louisville, KY 40292 USA.
[Sa Farinha, Carla Sofia e] DGS Directorate Gen Hlth, Lisbon, Portugal.
[Sa Farinha, Carla Sofia e] Univ Aberta, Lisbon, Portugal.
[Faro, Andre] Univ Fed Sergipe, Aracaju, Brazil.
[Farvid, Maryam S.] Massachusetts Gen Hosp, Mongan Inst Hlth Policy, Harvard MGH Ctr Genom, Vulnerable Populat & Hlth Disparities, Boston, MA USA.
[Feigin, Valery L.] Natl Inst Stroke & Appl Neurosci, Auckland, New Zealand.
[Ao, Braden J. Te] Auckland Univ Technol, Auckland, New Zealand.
[Fernandes, Jefferson G.] Inst Educ & Sci, German Hosp Oswaldo Cruz, Sao Paulo, Brazil.
[Fernandes, Joao C.] Queen Mary Univ London, William Harvey Res Inst, Barts & London Sch Med Dent, Ctr Expt Med Rheumatol, London, England.
[Fischer, Florian] Univ Bielefeld, Bielefeld, Germany.
[Foigt, Nataliya] Acad Med Sci, Inst Gerontol, Kiev, Ukraine.
[Fowkes, F. Gerry R.] Univ Edinburgh, Edinburgh, Midlothian, Scotland.
[Franklin, Richard C.] James Cook Univ, Townsville, Qld, Australia.
[Gankpe, Fortune Gbetoho] CHU Hassan II, Fes, Morocco.
[Garcia-Basteiro, Alberto L.] Manh Hlth Res Ctr, Manhica, Mozambique.
[Garcia-Basteiro, Alberto L.] Barcelona Inst Global Hlth, Barcelona, Spain.
[Gebremedhin, Amanuel Tesfay] Univ Munich, Munich, Germany.
[Geleijnse, Johanna M.] Wageningen Univ, Div Human Nutr, Wageningen, Netherlands.
[Jibat, Tariku] Wageningen Univ, Wageningen, Netherlands.
[Gibney, Katherine B.] Univ Melbourne, Peter Doherty Inst Infect & Immun, Melbourne, Vic, Australia.
[Gibney, Katherine B.] Royal Melbourne Hosp, Melbourne, Vic, Australia.
[Gillum, Richard F.; Mehari, Alem] Howard Univ, Coll Med, Washington, DC USA.
[Ginawi, Ibrahim Abdelmageem Mohamed] Univ Hail, Coll Med, Hail, Saudi Arabia.
[Hailu, Alemayehu Desalegne] Univ Addis Ababa, Sch Publ Hlth, Addis Ababa, Ethiopia.
[Giref, Ababi Zergaw; Haile, Demewoz; Jibat, Tariku] Univ Addis Ababa, Addis Ababa, Ethiopia.
[Giroud, Maurice] Univ Hosp Dijon, Dijon, France.
[Roba, Hirbo Shore] Haramaya Univ, Coll Hlth & Med Sci, Dawa, Ethiopia.
[Gishu, Melkamu Dedefo; Tura, Abera Kenay] Haramaya Univ, Dire Dawa, Ethiopia.
[Gishu, Melkamu Dedefo] Kersa Hlth & Demog Surveillance Syst, Harar, Ethiopia.
[Gona, Philimon] Univ Massachusetts, Boston, MA USA.
[Goodridge, Amador] Inst Invest Cient Serv Alta Tecnol, INDICASAT AIP, Ciudad Del Saber, Panama.
[Gopalani, Sameer Vali] Govt Federated States Micronesia, Dept Hlth & Social Affairs, Palikir, Micronesia.
[Gotay, Carolyn C.; Kissoon, Niranjan; Kopec, Jacek A.; Pourmalek, Farshad] Univ British Columbia, Vancouver, BC, Canada.
[Goto, Atsushi] Div Epidemiol, Ctr Publ Hlth Sci, Tokyo, Japan.
[Inoue, Manami] Natl Canc Ctr, Tokyo, Japan.
[Gupta, Rahul] West Virginia Bur Publ Hlth, Charleston, WV USA.
[Gupta, Rajeev] Eternal Heart Care Ctr & Res Inst, Jaipur, Rajasthan, India.
[Gupta, Vipin] Univ Delhi, Dept Anthropol, Delhi, India.
[Knudsen, Ann Kristin; Vollset, Stein Emil] Univ Bergen, Dept Global Publ Hlth & Primary Care, Bergen, Norway.
[Hailu, Alemayehu Desalegne; Norheim, Ole F.] Univ Bergen, Bergen, Norway.
[Hailu, Gessessew Bugssa] Kilte Awlaelo Hlth & Demog Surveillance Syst, Mekelle, Ethiopia.
[Halasa, Yara A.; Undurraga, Eduardo A.] Brandeis Univ, Waltham, MA USA.
[Hamadeh] Arabian Gulf Univ, Manama, Bahrain.
[Hamidi, Samer] Hamdan Bin Mohammed Smart Univ, Dubai, U Arab Emirates.
[Hammami, Mouhanad] Wayne Cty Dept Hlth & Human Serv, Detroit, MI USA.
[Handal, Alexis J.] Univ New Mexico, Albuquerque, NM USA.
[Hankey, Graeme J.] Univ Western Australia, Sch Med & Pharmacol, Perth, WA, Australia.
[Hankey, Graeme J.] Harry Perkins Inst Med Res, Nedlands, WA, Australia.
[Hankey, Graeme J.] Western Australian Neurosci Res Inst, Nedlands, WA, Australia.
[Harikrishnan, Sivadasanpillai] Sree Chitra Tirunal Inst Med Sci & Technol, Trivandrum, Kerala, India.
[Haro, Josep Maria] Parc Sanitari Sant Joan Deu CIBERSAM, Barcelona, Spain.
[Haro, Josep Maria] Univ Barcelona, Barcelona, Spain.
[Hay, Roderick J.] Int Fdn Dermatol, London, England.
[Hedayati, Mohammad T.] Mazandaran Univ Med Sci, Sch Med, Dept Med Mycol & Parasitol, Sari, Iran.
[Hoek, Hans W.] Univ Groningen, Univ Med Ctr Groningen, Dept Psychiat, Groningen, Netherlands.
[Tura, Abera Kenay] Univ Groningen, Univ Med Ctr Groningen, Groningen, Netherlands.
[Hoek, Hans W.] Columbia Univ, Dept Epidemiol, Mailman Sch Publ Hlth, New York, NY USA.
[Skirbekk, Vegard] Columbia Univ, New York, NY USA.
[Hoffman, Daniel J.] Rutgers State Univ, New Brunswick, NJ USA.
[Horino, Masako] Nevada Div Publ & Behav Hlth, Dept Hlth & Human Serv, Carson City, NV USA.
[Horita, Nobuyuki] Yokohama City Univ, Dept Pulmonol, Grad Sch Med, Yokohama, Kanagawa, Japan.
[Hosgood, H. Dean] Albert Einstein Coll Med, Bronx, NY USA.
[Hoy, Damian G.] Publ Hlth Div, Pacific Community, Noumea, New Caledonia.
[Hsairi, Mohamed] Salah Azaiz Inst, Dept Epidemiol, Tunis, Tunisia.
[Huang, Hsiang] Cambridge Hlth Alliance, Cambridge, MA USA.
[Iburg, Kim Moesgaard] Aarhus Univ, Aarhus, Denmark.
[Idrisov, Bulat T.] Boston Univ, Boston Med Ctr, Boston, MA USA.
[Kwan, Gene F.] Boston Univ, Sch Med, Boston, MA USA.
[Innos, Kaire] Natl Inst Hlth Dev, Tallinn, Estonia.
[Inoue, Manami] Univ Tokyo, Grad Sch Med, Tokyo, Japan.
[Kawakami, Norito] Univ Tokyo, Sch Publ Hlth, Tokyo, Japan.
[Shibuya, Kenji] Univ Tokyo, Tokyo, Japan.
[Jacobsen, Kathryn H.] George Mason Univ, Dept Global & Community Hlth, Fairfax, VA 22030 USA.
[Jayatilleke, Achala Upendra] Postgrad Inst Med, Colombo, Sri Lanka.
[Jayatilleke, Achala Upendra] Inst Violence & Injury Prevent, Colombo, Sri Lanka.
[Jeemon, Panniyammakal] Ctr Chron Dis Control, New Delhi, India.
[Jha, Vivekanand] George Inst Global Hlth India, New Delhi, India.
[Jiang, Guohong] Tianjin Ctr Dis Control & Prevent, Tianjin, Tianjin, Peoples R China.
[Jiang, Ying] Univ Occupat & Environm Hlth, Inst Ind Ecol Sci, Dept Hlth Dev, Kitakyushu, Fukuoka, Japan.
[Jimenez-Corona, Aida] Inst Ophthalmol Conde Valencia, Dept Ocular Epidemiol & Visual Hlth, Mexico City, DF, Mexico.
[Jimenez-Corona, Aida] Gen Directorate Epidemiol, Minist Hlth, Mexico City, DF, Mexico.
[Jonas, Jost B.] Heidelberg Univ, Med Fac Mannheim, Dept Ophthalmol, Mannheim, Germany.
[Kabir, Zubair] Univ Coll Cork, Cork, Ireland.
[Kajungu, Dan K.] Sante Stat Analyt Res Inst, Kampala, Uganda.
[Kajungu, Dan K.] Mildmay Uganda, Kampala, Uganda.
[Kalkonde, Yogeshwar] Action & Res Community Hlth, Soc Educ, Gadchiroli, India.
[Kamal, Ritul; Kesavachandran, Chandrasekharan Nair] CSIR Indian Inst Toxicol Res, Lucknow, Uttar Pradesh, India.
[She, Jun] Zhongshan Hosp, Dept Pulm Med, Shanghai, Peoples R China.
[Kan, Haidong] Fudan Univ, Shanghai, Peoples R China.
[Kandel, Amit] SUNY Buffalo, Buffalo, NY USA.
[Karch, Andre] Helmholtz Ctr Infect Res, Epidemiol & Stat Methods Res Grp, Braunschweig, Germany.
[Karch, Andre] German Ctr Infect Res, Hannover Braunschweig Site, Hannover, Germany.
[Karema, Corine Kakizi] Qual & Equity Hlth Care, Kigali, Rwanda.
[Karimkhani, Chante] Case Western Univ Hosp, Cleveland, OH USA.
[Kaul, Anil] Oklahoma State Univ, Tulsa, OK USA.
[Kazi, Dhruv S.] Univ Calif San Francisco, San Francisco, CA 94143 USA.
[Keiyoro, Peter Njenga] Inst Trop & Infect Dis, Nairobi, Kenya.
[Keiyoro, Peter Njenga] Sch Continuing & Distance Educ, Nairobi, Kenya.
[Lyons, Ronan A.] Farr Inst, Swansea, W Glam, Wales.
[Kemp, Andrew Haddon] Swansea Univ, Swansea, W Glam, Wales.
[Kengne, Andre Pascal; Matzopoulos, Richard; Wiysonge, Charles Shey] South African Med Res Council, Cape Town, South Africa.
[Matzopoulos, Richard] Univ Cape Town, Sch Publ Hlth & Family Med, Cape Town, South Africa.
[Stein, Dan J.] Univ Cape Town, Dept Psychiat, Cape Town, South Africa.
[Kengne, Andre Pascal; Mayosi, Bongani M.] Univ Cape Town, Cape Town, South Africa.
[Keren, Andre] Assuta Hosp, Assuta Hashalom, Tel Aviv, Israel.
[Khader, Yousef Saleh] Jordan Univ Sci & Technol, Irbid, Jordan.
[Khan, Ejaz Ahmad] Hlth Serv Acad, Islamabad, Pakistan.
[Khang, Young-Ho] Seoul Natl Univ, Coll Med, Seoul, South Korea.
[Won, Sungho] Seoul Natl Univ, Grad Sch Publ Hlth, Seoul, South Korea.
[Khoja, Tawfik Ahmed Muthafer] Execut Board Hlth Minist Council Cooperat Council, Riyadh, Saudi Arabia.
[Khubchandani, Jagdish] Ball State Univ, Muncie, IN 47306 USA.
[Kieling, Christian] Hosp Clin Porto Alegre, Porto Alegre, RS, Brazil.
[Kim, Cho-il] Korea Hlth Ind Dev Inst, Cheongju, South Korea.
[Kim, Daniel] Northeastern Univ, Dept Hlth Sci, Boston, MA USA.
[Kim, Yun Jin] Southern Univ Coll, Skudai, Malaysia.
[Knudsen, Ann Kristin; Vollset, Stein Emil] Ctr Dis Burden, Oslo, Norway.
[Skogen, Jens Christoffer] Norwegian Inst Publ Hlth, Dept Hlth Promot, Oslo, Norway.
[Savic, Miloje; Skirbekk, Vegard] Norwegian Inst Publ Hlth, Oslo, Norway.
[Kokubo, Yoshihiro] Natl Cerebral & Cardiovasc Ctr, Dept Prevent Cardiol, Suita, Osaka, Japan.
[Kolte, Dhaval] Brown Univ, Div Cardiol, Providence, RI USA.
[Koul, Parvaiz A.] Sherikashmir Inst Med Sci, Srinagar, Jammu & Kashmir, India.
[Koyanagi, Ai] Parc Sanitari Sant Joan Deu CIBERSAM, Res Dev Unit, Barcelona, Spain.
[Defo, Barthelemy Kuate] Univ Montreal, Dept Demog, Montreal, PQ, Canada.
[Defo, Barthelemy Kuate] Univ Montreal, Publ Hlth Res Inst, Montreal, PQ, Canada.
[Defo, Barthelemy Kuate] Univ Montreal, Dept Social & Prevent Med, Sch Publ Hlth, Montreal, PQ, Canada.
[Kuchenbecker, Ricardo S.] Univ Fed Rio Grande do Sul, Grad Studies Epidemiol, Porto Alegre, RS, Brazil.
[Bicer, Burcu Kucuk] Hacettepe Univ, Inst Publ Hlth, Ankara, Turkey.
[Kuipers, Ernst J.] Univ Med Ctr Rotterdam, Erasmus MC, Rotterdam, Netherlands.
[Lallukka, Tea; Shin, Rahman] Work Org, Work Disabil Prevent, Finnish Inst Occupat Hlth, Helsinki, Finland.
[Lallukka, Tea] Univ Helsinki, Dept Publ Hlth, Fac Med, Helsinki, Finland.
[Meretoja, Tuomo J.] Univ Helsinki, Helsinki, Finland.
[Latif, Asma Abdul] Lahore Coll Women Univ, Dept Zool, Lahore, Pakistan.
[Lavados, Pablo M.] Univ Desarrollo, Clin Alemana, Serv Neurol, Santiago, Chile.
[Lawrynowicz, Alicia Elena Beatriz] Inst Nacl Epidemiol Dr Juan H Jara, Mar Del Plata, Argentina.
[Leasher, Janet L.] Nova SE Univ, Coll Optometry, Ft Lauderdale, Ft Lauderdale, FL USA.
[Leung, Ricky] SUNY Albany, Albany, NY USA.
[Li, Yichong] San Francisco VA Med Ctr, San Francisco, CA USA.
[Lipshultz, Steven E.; Wilkinson, James D.] Wayne State Univ, Sch Med, Detroit, MI USA.
[Lipshultz, Steven E.] Childrens Hosp Michigan, Detroit, MI 48201 USA.
[Simard, Edgar P.] Emory Univ, Rollins Sch Publ Hlth, Atlanta, GA USA.
[Liu, Yang; Phillips, Michael Robert] Emory Univ, Atlanta, GA USA.
[Lloyd, Belinda K.] Turning Point, Eastern Hlth, Melbourne, Vic, Australia.
[Logroscino, Giancarlo] Univ Bari, Bari, Italy.
[Looker, Katharine J.; Rai, Dheeraj] Univ Bristol, Bristol, Avon, England.
[Lunevicius, Raimundas] Aintree Univ, Hosp Natl Hlth Serv Fdn Trust, Liverpool, Merseyside, England.
[Lunevicius, Raimundas] Univ Liverpool, Sch Med, Liverpool, Merseyside, England.
[El Razek, Hassan Magdy Abd] Mansoura Fac Med, Mansoura, Egypt.
Social Secur Org Res Inst, Tehran, Iran.
[Mckee, Martin] Erasmus Univ, Inst Hlth Policy & Management, Rotterdam, Netherlands.
[Malta, Deborah Carvalho] Univ Fed Minas Gerais, Belo Horizonte, MG, Brazil.
[Marcenes, Wagner] Kings Coll London, Div Populat & Patient Hlth, Inst Dent, London, England.
[Martinez-Raga, Jose] Univ Valencia, Univ Hosp Doctor Peset, Valencia, Spain.
[Martinez-Raga, Jose] CEU Cardenal Herrera Univ, Valencia, Spain.
[Mason-Jones, Amanda J.] Univ York, Dept Hlth Sci, York, N Yorkshire, England.
[Mckee, Martin; Murthy, Gudlavalleti Venkata Satyanarayana] London Sch Hyg Trop Med, London, England.
[Meaney, Peter A.] Univ Penn, Perelman Sch Med, Philadelphia, PA USA.
[Meaney, Peter A.] Childrens Hosp Philadelphia, Philadelphia, PA 19104 USA.
[Memiah, Peter] Univ Florida, Pensacola, FL USA.
[Memish, Ziad A.] Saudi Minist Hlth, Riyadh, Saudi Arabia.
[Memish, Ziad A.] Alfaisal Univ, Coll Med, Riyadh, Saudi Arabia.
[Mendoza, Walter] United Nations Populat Fund, Lima, Peru.
[Meretoja, Atte] Helsinki Univ Hosp, Dept Neurol, Helsinki, Finland.
[Meretoja, Tuomo J.] Helsinki Univ Hosp, Breast Surg Unit, Ctr Comprehens Canc, Helsinki, Finland.
[Mhimbira, Francis Apolinary] Ifakara Hlth Inst, Bagamoyo, Tanzania.
[Miller, Ted R.] Pacific Inst Res Evaluat, Calverton, MD USA.
[Miller, Ted R.] Curtin Univ, Ctr Populat Hlth, Perth, WA, Australia.
[Mills, Edward J.] Univ Ottawa, Ottawa, ON, Canada.
[Mirrakhimov, Erkin M.] Kyrgyz State Med Acad, Bishkek, Kyrgyzstan.
[Mirrakhimov, Erkin M.] Natl Ctr Cardiol & Internal Dis, Bishkek, Kyrgyzstan.
[Mohammad, Karzan Abdulmuhsin] Univ Salahaddin, Erbil, Iraq.
[Mohammadi, Alireza] Baqiyatallah Univ Med Sci, Neurosci Res Ctr, Tehran, Iran.
[Mohammed, Shafiu] Ahmadu Bello Univ, Hlth Syst & Policy Res Unit, Zaria, Nigeria.
[Monasta, Lorenzo; Montico, Marcella; Ronfani, Luca] IRCCS Burlo Garofolo, Inst Maternal & Child Hlth, Trieste, Italy.
[Moradi-Lakeh, Maziar] Iran Univ Med Sci, Dept Community Med, Gastrointestinal & Liver Dis Res Ctr, Prevent Med & Publ Hlth Res Ctr, Tehran, Iran.
[Werdecker, Andrea] Competence Ctr Mortal Follow Up German Natl Cohor, Wiesbaden, Germany.
[Mueller, Ulrich O.; WestermaM, Ronny] Fed Inst Populat Res, Wiesbaden, Germany.
[Murdoch, Michele E.] West Herts Hosp NHS Trust, Watford, England.
[Murthy, Gudlavalleti Venkata Satyanarayana] Indian Inst Publ Hlth, Gurgaon, India.
[Dhillon, Preet K.; Zodpey, Sanjay] Publ Hlth Fdn India, Gurgaon, India.
[Nachega, Jean B.] Univ Pittsburgh, Grad Sch Publ Hlth, Pittsburgh, PA USA.
[Nachega, Jean B.; Seedat, Soraya; Wiysonge, Charles Shey] Univ Stellenbosch, Cape Town, South Africa.
[Nachega, Jean B.] Johns Hopkins Univ, Bloomberg Sch Publ Hlth, Baltimore, MD USA.
[Tran, Bach Xuan] Johns Hopkins Univ, Baltimore, MD USA.
[Naheed, Aliya] Int Ctr Diarrhoeal Dis Res, Dhaka, Bangladesh.
[Naldi, Luigi; Remuzzi, Giuseppe] Azienda Osped Papa Giovanni XXIII, Bergamo, Italy.
[Nangia, Vinay] Suraj Eye Inst, Nagpur, Maharashtra, India.
[Ngalesoni, Frida Namnyak] Minist Hlth & Social Welf, Dar Es Salaam, Tanzania.
[Le Nguyen, Quyen] Duy Tan Univ, Inst Global Hlth Innovat, Da Nang, Vietnam.
[Pete, Patrick Martial Nkamedjie] Inst Res, Socioecon Dev & Commun, Yaounde, Cameroon.
[Nolla, Joan M.] Hosp Univ Bellvitge, Lhospitalet De Llobregat, Spain.
[Norman, Rosana E.] Queensland Univ Technol, Inst Hlth & Biomed Innovat, Brisbane, Qld, Australia.
[Obermeyer, Carla Makhlouf] Amer Univ Beirut, Ctr Res Populat & Hlth, Fac Hlth Sci, Beirut, Lebanon.
[Ogbo, Felix Akpojene] Univ Western Sydney, Ctr Hlth Res, Sydney, NSW, Australia.
[Oh, In-Hwan] Kyung Hee Univ, Sch Med, Dept Prevent Med, Seoul, South Korea.
[Oladimeji, Olanrewaju] Human Sci Res Council, Durban, South Africa.
[Oladimeji, Olanrewaju; Sartorius, Benn] Univ KwaZulu Natal, Durban, South Africa.
[Olivares, Pedro R.] Univ Autonoma Chile, Talca, Chile.
[Olusanya, Bolajoko Olubukunola; Olusanya, Jacob Olusegun] Ctr Healthy Start Initiat, Lagos, Nigeria.
[Oren, Eyal] Univ Arizona, Tucson, AZ USA.
[Ortiz, Alberto] IIS Fdn Jimenez Diaz UAM, Madrid, Spain.
[Ota, Erika] Lukes Int Univ, Tokyo, Japan.
[Schutte, Aletta E.] HART, Mafikeng, South Africa.
[Oyekale, Abayomi Samuel] Hypertens NorthWest Univ, Mafikeng, South Africa.
[Pa, Mahesh] JSS Univ, JSS Med Coll, Mysore, Karnataka, India.
[Park, Eun-Kee] Kosin Univ, Dept Med Human & Social Med, Coll Med, Busan, South Korea.
[Patten, Scott B.] Univ Calgary, Dept Community Hlth Sci, Calgary, AB, Canada.
[Tonelli, Marcello] Univ Calgary, Calgary, AB, Canada.
[Pedro, Joao Mario] Hlth Res Ctr Angola, Caxito, Angola.
[Pereira, David M.] Univ Porto, REQUIMTE LAQV, Lab Farm, Dept Quim,Fac Farm, Oporto, Portugal.
[Perico, Norberto; Remuzzi, Giuseppe] IRCCS Ist Ric Farmacol Mario Negri, Bergamo, Italy.
[Pesudovs, Konrad] Flinders Univ S Australia, Adelaide, SA, Australia.
[Petzold, Max] Univ Witwatersrand, Johannesburg, South Africa.
[Phillips, Michael Robert] Shanghai Jiao Tong Univ, Sch Med, Shanghai, Peoples R China.
[Pillay, Julian David] Durban Univ Technol, Durban, South Africa.
[Plass, Dietrich] Exposure Assessment & Environm Hlth Indicators, German Environm Agcy, Berlin, Germany.
[Polinder, Suzanne] Erasmus MC, Dept Publ Hlth, Rotterdam, Netherlands.
[Prasad, Noela M.] Fred Hollows Fdn, Sydney, NSW, Australia.
[Prasad, Noela M.] Ctr Eye Res Australia, Melbourne, Vic, Australia.
[Qorbani, Mostafa] Alborz Univ Med Sci, Sch Med, Dept Community Med, Karaj, Iran.
[Radfar, Amir] AT Still Univ, Kirksville, MO USA.
[Rafay, Anwar] Contech Sch Publ Hlth, Lahore, Pakistan.
[Rahman, Mahfuzar] Res & Evaluat Div, BRAC, Dhaka, Bangladesh.
[Rahman, Sajjad Ur] Hamad Med Corp, Doha, Qatar.
[Rai, Rajesh Kumar] Soc Hlth & Demog Surveillance, Suri, India.
[Rajsic, Sasa] UMIT, ERAWEB Program, Hall In Tirol, Austria.
[Raju, Murugesan] Univ Missouri, Columbia, MO USA.
[Ranganathan, Kavitha] Univ Michigan Hlth Syst, Ann Arbor, MI USA.
[Refaat, Amany H.] Walden Univ, Minneapolis, MN USA.
[Refaat, Amany H.] Suez Canal Univ, Ismailia, Egypt.
[Remuzzi, Giuseppe] Univ Milan, Dept Biomed & Clin Sci Sacco L, Milan, Italy.
[Ribeiro, Antonio L.] Univ Fed Minas Gerais, Hosp Clin, Belo Horizonte, MG, Brazil.
[Ricci, Stefano] UO Neurol USL Umbria 1, Citta Di Castello, Italy.
[Rojas-Rueda, David] Inst Salud Global Barcelona, Barcelona, Spain.
[Roshandel, Gholamreza] Golestan Univ Med Sci, Golestan Res Ctr Gastroenterol & Hepatol, Gorgan, Iran.
[Sackey, Ben Benasco] World Hlth Org, Accra, Ghana.
[Sanabria, Juan R.] Marshall Univ, Edwards Sch Med J, Huntington, WV USA.
[Sanabria, Juan R.] Case Western Reserve Univ, Cleveland, OH USA.
[Dolores Sanchez-Nino, Maria] IIS Fdn Jimenez Diaz, Madrid, Spain.
[Sarmiento-Suarez, Rodrigo] Univ Ciencias Aplicadas Ambient, Bogota, Colombia.
[Sawhney, Monika] Marshall Univ, Huntington, WV USA.
[Schneider, Ione J. C.; Santos Silva, Diego Augusto] Univ Fed Santa Catarina, Florianopolis, SC, Brazil.
[Schutte, Aletta E.] South African Med Res Council, Potchefstroom, South Africa.
[Schwebel, David C.; Singh, Jasvinder A.] Univ Alabama Birmingham, Birmingham, AL USA.
[Shahraz, Saeid] Tufts Med Ctr, Boston, MA USA.
[Shaikh, Masood Ali] Independent Consultant, Karachi, Pakistan.
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[Shigematsu, Mika] Sandia Natl Labs, Albuquerque, NM USA.
[Shin, Min-Jeong] Korea Univ, Dept Publ Hlth Sci, Grad Sch, Seoul, South Korea.
[Yoon, Seok-Jun] Korea Univ, Dept Prevent Med, Coll Med, Seoul, South Korea.
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[Silverberg, Jonathan I.] Northwestern Univ, Feinberg Sch Med, Chicago, IL USA.
[Yan, Yuichiro] Northwestern Univ, Dept Prevent Med, Chicago, IL USA.
[Singh, Prashant Kumar] Inst Human Dev, New Delhi, India.
[Skogen, Jens Christoffer] Alcohol & Drug Res Western Norway, Stavanger, Norway.
[Soreide, Kjetil] Stavanger Univ Hosp, Stavanger, Norway.
[Sreeramareddy, Chandrashekhar T.] Int Med Univ, Dept Community Med, Kuala Lumpur, Malaysia.
[Stathopoulou, Vasiliki] Attikon Univ Hosp, Athens, Greece.
[Steel, Nicholas] Univ Anglia, Norwich, Norfolk, England.
[Stein, Dan J.] S African MRC, Unit Anxiety Stress Dis, Cape Town, South Africa.
[Stein, Murray B.] Univ Calif San Diego, San Diego, CA USA.
[Steiner, Timothy J.; Stovner, Lars Jacob] Norwegian Univ Sci & Technol, Dept Neurosci, Trondheim, Norway.
[Stovner, Lars Jacob] St Olays Hosp, Norwegian Advisory Unit Headache, Trondheim, Norway.
[Stroumpoulis, Konstantinos] Alexandra Gen Hosp Athens, Athens, Greece.
[Stroumpoulis, Konstantinos] Ctr Hosp Publ Cotentin, Cherbourg, France.
[Sunguya, Bruno F.] Muhimbili Univ Hlth & Allied Sci, Dar Es Salaam, Tanzania.
[Swaminathan, Soumya] Indian Council Med Res, New Delhi, India.
[Sykes, Bryan L.] Univ Calif Irvine, Dept Criminol Law & Soc Sociol & Publ Hlth, Irvine, CA USA.
[Tanne, David] Chaim Sheba Med Ctr, Tel Hashomer, Israel.
[Tanne, David] Tel Aviv Univ, Tel Aviv, Israel.
[Tavakkoli, Mohammad] New York Med Coll, Valhalla, NY USA.
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[Terkawi, Abdullah Sulieman] Cleveland Clin, Outcomes Res Consortium, Cleveland, OH USA.
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[Tessema, Gizachew Assefa] Univ Gondar, Gondar, Ethiopia.
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[Thomson, Alan J.] Adapt Knowledge Management, Victoria, BC, Canada.
[Thorne-Lyman, Andrew L.] WorldFish, George Town, Malaysia.
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[Topor-Madry, Roman] Wroclaw Med Univ, Fac Hlth Sci, Wroclaw, Poland.
[Topouzis, Fotis] Aristotle Univ Thessaloniki, Thessaloniki, Greece.
[Tran, Bach Xuan] Hanoi Med Univ, Hanoi, Vietnam.
[Dimbuene, Zacharie Tsala] Univ Kinshasa, Fac Econ & Management, Dept Populat Sci & Dev, Kinshasa, Congo.
[Dimbuene, Zacharie Tsala] African Populat & Hlth Res Ctr, Nairobi, Kenya.
[Tsilimbaris, Miltiadis] Univ Crete, Dept Med, Iraklion, Greece.
[Tyrovolas, Stefanos] Univ Barcelona, Parc Sanitari Sant Joan Deu, Fundacio Sant Joan Deu, CIBERSAM, Barcelona, Spain.
[Ukwaja, Kingsley N.] Fed Teaching Hosp, Dept Internal Med, Abakaliki, Nigeria.
[Uneke, Chigozie Jesse] Ebonyi State Univ, Abakaliki, Nigeria.
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[Zaki, Maysaa El Sayed] Mansoura Univ, Fac Med, Mansoura, Egypt.
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RP Murray, CJL (reprint author), 2301 5th Ave,Suite 600, Seattle, WA 98121 USA.
EM cjlm@uw.edu
RI Lotufo, Paulo/A-9843-2008; Karch, Andre/D-6973-2017; Patten,
Scott/B-4434-2011; Franklin, Richard/H-1731-2012; Giussani,
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David/M-9286-2013; Ribeiro, Antonio/C-2707-2009; Gishu, Melkamu
Dedefo/C-3747-2017; Alsharif, Ubai/C-6527-2017; Tonelli,
Marcello/B-3028-2009; Salomon, Joshua/D-3898-2009; Monasta,
Lorenzo/B-1388-2012; Hankey, Graeme /H-4968-2014; Patton,
George/B-5246-2013; Malta, Deborah/H-7880-2012; Martinez-Raga,
Jose/B-6251-2017; Majdan, Marek/K-5017-2012; Weiderpass,
Elisabete/M-4029-2016; Amini, Heresh/B-3076-2010
OI Mirrakhimov, Erkin/0000-0003-2982-6108; Degenhardt,
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Jacobsen, Kathryn/0000-0002-4198-6246; Bernabe,
Eduardo/0000-0002-1858-3713; Piel, Frederic B./0000-0001-8131-7728;
Hoek, Hans/0000-0001-6353-5465; NORMAN, ROSANA/0000-0002-9742-1957;
Altirkawi, Khalid/0000-0002-7331-4196; Alkerwi,
Ala'a/0000-0002-7448-3936; Ahmad Kiadaliri,
Aliasghar/0000-0002-4254-9099; Leung, Ricky/0000-0002-2852-6771;
Kieling, Christian/0000-0001-7691-4149; Gething,
Peter/0000-0001-6759-5449; Rai, Dheeraj/0000-0002-7239-3523; Taylor,
Hugh/0000-0002-9437-784X; Pishgar, Farhad/0000-0003-0703-8442; Kemp,
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Karch, Andre/0000-0003-3014-8543; Patten, Scott/0000-0001-9871-4041;
Franklin, Richard/0000-0003-1864-4552; Abbas, Kaja/0000-0003-0563-1576;
Pereira, David/0000-0003-0384-7592; Sreeramareddy,
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Gelin/0000-0002-6194-0341; Al-Aly, Ziyad/0000-0002-2600-0434;
Heydarpour, Pouria/0000-0001-5644-7555; Vlassov,
Vasiliy/0000-0001-5203-549X; Ribeiro, Antonio/0000-0002-2740-0042;
Gishu, Melkamu Dedefo/0000-0002-3466-1232; Alsharif,
Ubai/0000-0002-4024-3950; Salomon, Joshua/0000-0003-3929-5515; Monasta,
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Patton, George/0000-0001-5039-8326; Malta, Deborah/0000-0002-8214-5734;
Martinez-Raga, Jose/0000-0002-2856-6562; Majdan,
Marek/0000-0001-8037-742X; Weiderpass, Elisabete/0000-0003-2237-0128;
Amini, Heresh/0000-0002-4825-1322
FU Bill AMP; Melinda Gates Foundation
FX Bill & Melinda Gates Foundation.
NR 65
TC 13
Z9 13
U1 62
U2 62
PU ELSEVIER SCIENCE INC
PI NEW YORK
PA 360 PARK AVE SOUTH, NEW YORK, NY 10010-1710 USA
SN 0140-6736
EI 1474-547X
J9 LANCET
JI Lancet
PD OCT 8
PY 2016
VL 388
IS 10053
BP 1603
EP 1658
PG 56
WC Medicine, General & Internal
SC General & Internal Medicine
GA DY7BU
UT WOS:000385285000009
ER
PT J
AU Forouzanfar, MH
Afshin, A
Alexander, LT
Anderson, HR
Bhutta, ZA
Biryukov, S
Brauer, M
Burnett, R
Cercy, K
Charlson, FJ
Cohen, AJ
Dandona, L
Estep, K
Ferrari, AJ
Frostad, JJ
Fullman, N
Gething, PW
Godwin, WW
Griswold, M
Kinfu, Y
Kyu, HH
Larson, HJ
Liang, X
Lim, SS
Liu, PY
Lopez, AD
Lozano, R
Marczak, L
Mensah, GA
Mokdad, AH
Moradi-Lakeh, M
Naghavi, M
Neal, B
Reitsma, MB
Roth, GA
Salomon, JA
Sur, PJ
Vos, T
Wagner, JA
Wang, H
Zhao, Y
Zhou, M
Aasvang, GM
Abajobir, AA
Abate, KH
Abbafati, C
Abbas, KM
Abd-Allah, F
Abdulle, AM
Abera, SF
Abraham, B
Abu-Raddad, LJ
Abyu, GY
Adebiyi, AO
Adedeji, IA
Ademi, Z
Adou, AK
Adsuar, JC
Agardh, EE
Agarwal, A
Agrawal, A
Kiadaliri, AA
Ajala, ON
Akinyemiju, TF
Al-Aly, Z
Alam, K
Alam, NKM
Aldhahri, SF
Aldridge, RW
Alemu, ZA
Ali, R
Alkerwi, A
Alla, F
Allebeck, P
Alsharif, U
Altirkawi, KA
Martin, EA
Alvis-Guzman, N
Amare, AT
Amberbir, A
Amegah, AK
Amini, H
Ammar, W
Amrock, SM
Andersen, HH
Anderson, BO
Antonio, CAT
Anwar, P
Arnlov, J
Al Artaman
Asayesh, H
Asghar, RJ
Assadi, R
Atique, S
Avokpaho, EFGA
Awasthi, A
Quintanilla, BPA
Azzopardi, P
Bacha, U
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Bahit, MC
Balakrishnan, K
Barac, A
Barber, RM
Barker-Collo, SL
Barnighausen, T
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Bans, C
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Borschmann, R
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Bourne, RRA
Brainin, M
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Breitborde, NJK
Brenner, H
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Butt, ZA
Cahill, LE
Calabria, B
Campos-Nonato, IR
Cardenas, R
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Casey, DC
Castaneda-Oquela, CA
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Castro, RE
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Christensen, H
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Cornaby, L
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das Neves, J
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Gutierrez, RA
Haagsma, JA
Hafezi-Nejad, N
Haile, D
Hailu, GB
Halasa, YA
Hamadeh, RR
Hamidi, S
Handal, AJ
Hankey, GJ
Hao, YT
Harb, HL
Harikrishnan, S
Haro, JM
Hassanvand, MS
Hassen, TA
Havmoeller, R
Heredia-Pi, IB
Hernandez-Llanes, NF
Heydarpour, P
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Htet, AS
Hu, G
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Husseini, A
Hutchings, SJ
Huybrechts, I
Iburg, KM
Idrisov, BT
Ileanu, BV
Inoue, M
Jacobs, TA
Jacobsen, KH
Jahanmehr, N
Jakovljevic, MB
Jansen, HAFM
Jassal, SK
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Jayatilleke, AU
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Johnson, CO
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Karimkhani, C
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Khang, YH
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Khoja, TAM
Khubchandani, J
Kieling, C
Kim, CI
Kim, D
Kimokoti, RW
Kissoon, N
Kivipelto, M
Knibbs, LD
Kokubo, Y
Kopec, JA
Koul, PA
Koyanagi, A
Kravchenko, M
Kromhout, H
Krueger, H
Ku, T
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Kuchenbecker, RS
Bicer, BK
Kuipers, EJ
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Lalloo, R
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Larsson, A
Latif, AA
Lawrynowicz, AEB
Leasher, JL
Leigh, J
Leung, J
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Li, XH
Li, YC
Liang, J
Liu, SW
Lloyd, BK
Logroscino, G
Lotufo, PA
Lunevicius, R
Maclntyre, M
Mahdavi, M
Majdan, M
Majeed, A
Malekzadeh, R
Malta, DC
Manamo, WAA
Mapoma, CC
Marcenes, W
Martin, RV
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Masiye, F
Matsushita, K
Matzopoulos, R
Mayosi, BM
McGrath, JJ
McKee, M
Meaney, PA
Medina, C
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CA GBD 2015 Risk Factors
TI Global, regional, and national comparative risk assessment of 79
behavioural, environmental and occupational, and metabolic risks or
clusters of risks, 1990-2015: a systematic analysis for the Global
Burden of Disease Study 2015
SO LANCET
LA English
DT Article
ID ISCHEMIC-HEART-DISEASE; DOSE-RESPONSE METAANALYSIS; BODY-MASS INDEX;
ALCOHOL-CONSUMPTION; CARDIOVASCULAR-DISEASE; BLOOD-PRESSURE;
NONCOMMUNICABLE DISEASES; ECONOMIC-DEVELOPMENT; COST-EFFECTIVENESS;
REDUCED MORTALITY
AB Background The Global Burden of Diseases, Injuries, and Risk Factors Study 2015 provides an up-to-date synthesis of the evidence for risk factor exposure and the attributable burden of disease. By providing national and subnational assessments spanning the past 25 years, this study can inform debates on the importance of addressing risks in context.
Methods We used the comparative risk assessment framework developed for previous iterations of the Global Burden of Disease Study to estimate attributable deaths, disability-adjusted life-years (DALYs), and trends in exposure by age group, sex, year, and geography for 79 behavioural, environmental and occupational, and metabolic risks or clusters of risks from 1990 to 2015. This study included 388 risk-outcome pairs that met World Cancer Research Fund-defined criteria for convincing or probable evidence. We extracted relative risk and exposure estimates from randomised controlled trials, cohorts, pooled cohorts, household surveys, census data, satellite data, and other sources. We used statistical models to pool data, adjust for bias, and incorporate covariates. We developed a metric that allows comparisons of exposure across risk factors-the summary exposure value. Using the counterfactual scenario of theoretical minimum risk level, we estimated the portion of deaths and DALYs that could be attributed to a given risk. We decomposed trends in attributable burden into contributions from population growth, population age structure, risk exposure, and risk-deleted cause-specific DALY rates. We characterised risk exposure in relation to a Socio-demographic Index (SDI).
Findings Between 1990 and 2015, global exposure to unsafe sanitation, household air pollution, childhood underweight, childhood stunting, and smoking each decreased by more than 25%. Global exposure for several occupational risks, high body-mass index (BMI), and drug use increased by more than 25% over the same period. All risks jointly evaluated in 2015 accounted for 57.8% (95% CI 56.6-58.8) of global deaths and 41.2% (39.8-42.8) of DALYs. In 2015, the ten largest contributors to global DALYs among Level 3 risks were high systolic blood pressure (211.8 million [192.7 million to 231.1 million] global DALYs), smoking (148.6 million [134.2 million to 163.1 million]), high fasting plasma glucose (143.1 million [125.1 million to 163.5 million]), high BMI (120.1 million [83.8 million to 158.4 million]), childhood undernutrition (113.3 million [103.9 million to 123.4 million]), ambient particulate matter (103.1 million [90.8 million to 115.1 million]), high total cholesterol (88.7 million [74.6 million to 105.7 million]), household air pollution (85.6 million [66.7 million to 106.1 million]), alcohol use (85.0 million [77.2 million to 93.0 million]), and diets high in sodium (83.0 million [49.3 million to 127.5 million]). From 1990 to 2015, attributable DALYs declined for micronutrient deficiencies, childhood undernutrition, unsafe sanitation and water, and household air pollution; reductions in risk-deleted DALY rates rather than reductions in exposure drove these declines. Rising exposure contributed to notable increases in attributable DALYs from high BMI, high fasting plasma glucose, occupational carcinogens, and drug use. Environmental risks and childhood undernutrition declined steadily with SDI; low physical activity, high BMI, and high fasting plasma glucose increased with SDI. In 119 countries, metabolic risks, such as high BMI and fasting plasma glucose, contributed the most attributable DALYs in 2015. Regionally, smoking still ranked among the leading five risk factors for attributable DALYs in 109 countries; childhood underweight and unsafe sex remained primary drivers of early death and disability in much of sub-Saharan Africa.
Interpretation Declines in some key environmental risks have contributed to declines in critical infectious diseases. Some risks appear to be invariant to SDI. Increasing risks, including high BMI, high fasting plasma glucose, drug use, and some occupational exposures, contribute to rising burden from some conditions, but also provide opportunities for intervention. Some highly preventable risks, such as smoking, remain major causes of attributable DALYs, even as exposure is declining. Public policy makers need to pay attention to the risks that are increasingly major contributors to global burden. Copyright (C) The Author(s). Published by Elsevier Ltd.
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[Mock, Charles N.] Univ Washington, Harborview Injury Prevent & Res Ctr, Seattle, WA 98195 USA.
[Anderson, Benjamin O.; Futran, Neal D.] Univ Washington, Seattle, WA 98195 USA.
[Anderson, H. Ross] St Georges Univ London, Populat Hlth Res Inst, London, England.
[Bhutta, Zulficiar A.] Aga Khan Univ, Ctr Excellence Women & Child Hlth, Karachi, Pakistan.
[Nisar, Muhammad Imran] Aga Khan Univ, Karachi, Pakistan.
[Bhutta, Zulficiar A.] Hosp Sick Children, Ctr Global Child Hlth, Toronto, ON, Canada.
[Krueger, Hans] Univ British Columbia, Sch Populat & Publ Hlth, Vancouver, BC, Canada.
[Gotay, Carolyn C.; Kissoon, Niranjan; Kopec, Jacek A.; Pourmalek, Farshad] Univ British Columbia, Vancouver, BC, Canada.
[Burnett, Richard] Hlth Canada, Ottawa, ON, Canada.
[Charlson, Fiona J.; Ferrari, Alize J.; Erskine, Holly E.; Knibbs, Luke D.; Leung, Janni; Santomauro, Damian F.; Veerman, J. Lennert; Whiteford, Harvey A.] Univ Queensland, Sch Publ Hlth, Brisbane, Qld, Australia.
[Lalloo, Ratilal] Univ Queensland, Sch Dent, Brisbane, Qld, Australia.
[Scott, James G.] Univ Queensland, Clin Res Ctr, Brisbane, Qld, Australia.
[Alam, Noore K. M.; Gouda, Hebe N.; Guo, Yuming; McGrath, John J.] Univ Queensland, Brisbane, Qld, Australia.
[Charlson, Fiona J.; Ferrari, Alize J.; Erskine, Holly E.; Leung, Janni; Santomauro, Damian F.; Whiteford, Harvey A.] Queensland Ctr Mental Hlth Res, Brisbane, Qld, Australia.
[Cohen, Aaron J.] Hlth Effects Inst, Boston, MA USA.
[Jeemon, Panniyammakal] Publ Hlth Fdn India, Ctr Control Chron Condit, New Delhi, India.
[Dandona, Lalit; Dandona, Rakhi; Goenka, Shifalika; Kumar, G. Anil] Publ Hlth Fdn India, New Delhi, India.
[Gething, Peter W.] Univ Oxford, Dept Zool, Oxford, England.
[Bisanzio, Donal; Deribew, Amare] Univ Oxford, Nuffield Dept Med, Oxford, England.
[Darby, Sarah C.] Univ Oxford, Clin Trial Serv Unit, Oxford, England.
[Ali, Raghib; Bennett, Derrick A.; Jha, Vivekanand] Univ Oxford, Oxford, England.
[Kinfu, Yohannes] Univ Canberra, Fac Hlth, Ctr Res & Act Publ Hlth, Canberra, ACT, Australia.
[Larson, Heidi J.] London Sch Hyg & Trop Med, Dept Infect Dis Epidemiol, London, England.
[McKee, Martin; Murthy, Gudlavalleti Venkata Satyanarayana; Pearce, Neil; Stockl, Heidi] London Sch Hyg & Trop Med, London, England.
[Zhou, Maigeng; Duan, Leilei; Jin, Ye; Li, Yichong; Liu, Shiwei; Wang, Linhong; Ye, Pengpeng] Chinese Ctr Dis Control & Prevent, Ctr Chron & Noncommunicable Dis Control & Prevent, Beijing, Peoples R China.
[Liang, Xiaofeng] Chinese Ctr Dis Control & Prevent, Beijing, Peoples R China.
[Lopez, Alan D.] Univ Melbourne, Melbourne Sch Populat & Global Hlth, Melbourne, Vic, Australia.
[Azzopardi, Peter; Patton, George C.] Univ Melbourne, Dept Paediat, Melbourne, Vic, Australia.
[Meretoja, Atte] Univ Melbourne, Dept Med, Melbourne, Vic, Australia.
[Alam, Khurshid; Azzopardi, Peter; Borschmann, Rohan; Colquhoun, Samantha M.; Patton, George C.; Weintraub, Robert G.] Univ Melbourne, Murdoch Childrens Res Inst, Melbourne, Vic, Australia.
[Szoeke, Cassandra E. I.] Univ Melbourne, Inst Hlth & Ageing, Melbourne, Vic, Australia.
[Ademi, Zanfina; Alam, Khurshid; Borschmann, Rohan; Colquhoun, Samantha M.; Taylor, Hugh R.; Weintraub, Robert G.] Univ Melbourne, Melbourne, Vic, Australia.
Natl Inst Publ Hlth, Natl Council Sci & Technol, Cuernavaca, Morelos, Mexico.
[Lozano, Rafael; Barquera, Simon; Ricardo Campos-Nonato, Ismael; Cuevas-Nasu, Lucia; Filipa de Castro, E.; De la Cruz-Gongora, Vanessa; Gomez-Dantes, Hector; Beatriz Heredia-Pi, Ileana; Medina, Catalina; Montanez Hernandez, Julio Cesar; Razo Garcia, Christian Aspacia; Rivera, Juan A.; Rodriguez-Ramirez, Sonia; Sanchez-Pimienta, Tania G.; Servan-Mori, Edson E.] Natl Inst Publ Hlth, Cuernavaca, Morelos, Mexico.
[Mensah, George A.] NHLBI, Ctr Translat Res & Implementat Sci, NIH, Bldg 10, Bethesda, MD 20892 USA.
[Hoffman, Howard J.] Natl Inst Deafness & Other Commun Disorders, Epidemiol & Stat Program, NIH, Bethesda, MD USA.
[Neal, Bruce] George Inst Global Hlth, Sydney, NSW, Australia.
[Driscoll, Tim R.] Univ Sydney, Sydney Sch Publ Hlth, Sydney, NSW, Australia.
[Neal, Bruce; Alam, Khurshid; Kemp, Andrew Haddon; Leigh, James; Mekonnen, Alemayehu B.] Univ Sydney, Sydney, NSW, Australia.
[Neal, Bruce] Royal Prince Alfred Hosp, Sydney, NSW, Australia.
[Bhatt, Samir] Imperial Coll London, Dept Infect Dis Epidemiol, London, England.
[Piel, Frederic B.; Rodriguez, Anna] Imperial Coll London, Dept Epidemiol & Biostat, Sch Publ Hlth, London, England.
[Neal, Bruce; Hutchings, Sally J.; Majeed, Azeem; Soljak, Michael] Imperial Coll London, London, England.
[Salomon, Joshua A.] Harvard Univ, Dept Global Hlth & Populat, Boston, MA 02115 USA.
[Thorne-Lyman, Andrew L.] Harvard Univ, Dept Nutr, Boston, MA 02115 USA.
[Ajala, Oluremi N.; Baernighausen, Till; Cahill, Leah E.; Ricardo Campos-Nonato, Ismael; Ding, Eric L.; Farvid, Maryam S.; Khatibzadeh, Shahab; Wagner, Gregory R.] Harvard Univ, Harvard TH Chan Sch Publ Hlth, Boston, MA 02115 USA.
[Shrime, Mark G.] Harvard Univ, Harvard Med Sch, Boston, MA 02115 USA.
[Fitchett, Joseph R. A.] Harvard Univ, Boston, MA 02115 USA.
[Vollset, Stein Emil] Norwegian Inst Publ Hlth, Ctr Dis Burden, Oslo, Norway.
[Aasvang, Gunn Marit; Savic, Miloje] Norwegian Inst Publ Hlth, Oslo, Norway.
[Abate, Kalkidan Hassen; Gebrehiwot, Tsegaye Tewelde; Gebremedhin, Amanuel Tesfay] Jimma Univ, Jimma, Ethiopia.
[Abbafati, Cristiana] Univ Roma La Sapienza, Rome, Italy.
[Abbas, Kaja M.] Virginia Tech, Blacksburg, VA USA.
[Abd-Allah, Foad] Cairo Univ, Dept Neurol, Cairo, Egypt.
[Abdulle, Abdishakur M.] New York Univ Abu Dhabi, Abu Dhabi, U Arab Emirates.
[Abera, Semaw Ferede] Mekelle Univ, Sch Publ Hlth, Coll Hlth Sci, Mekelle, Ethiopia.
[Melaku, Yohannes Adama] Mekelle Univ, Sch Publ Hlth, Mekelle, Ethiopia.
[Abyu, Gebre Yitayih; Betsu, Balem Demtsu; Hailu, Gessessew Bugssa; Tekle, Dejen Yemane; Yalew, Ayalnesh Zemene] Mekelle Univ, Mekelle, Ethiopia.
[Abera, Semaw Ferede] Kilte Awlaelohlth & Demog Surveillance Site, Mekelle, Ethiopia.
[Abera, Semaw Ferede] Univ Hohenheim, Food Secur & Inst Biol Chem & Nutr, Stuttgart, Germany.
[Abraham, Biju] NM SM Govt Coll Kalpetta, Kalpetta, Kerala, India.
[Abu-Raddad, Laith J.] Weill Cornell Med Coll Qatar, Infect Dis Epidemiol Grp, Doha, Qatar.
[Adebiyi, Akindele Olupelumi] Univ Ibadan, Coll Med, Ibadan, Nigeria.
[Adebiyi, Akindele Olupelumi] Univ Coll Hosp, Ibadan, Nigeria.
[Adedeji, Isaac Akinkunmi] Olabisi Onabanjo Univ, Ago Iwoye, Nigeria.
[Ademi, Zanfina; Fuerst, Thomas] Univ Basel, Basel, Switzerland.
[Adou, Arsene Kouablan] Assoc Ivoirienne Bien Etre Familial, Abidjan, Cote Ivoire.
[Adsuar, Jose C.] Univ Extremadura, Caceres, Spain.
[Agardh, Emilie Elisabet] Inst Publ Hlth Sci, Stockholm, Sweden.
[Rehm, Jurgen] Univ Toronto, Dalla Lana Sch Publ Hlth, Toronto, ON, Canada.
[Badawi, Alaa] Univ Toronto, Dept Nutr Sci, Fac Med, Toronto, ON, Canada.
[Popova, Svetlana] Univ Toronto, Ctr Addict & Mental Hlth, Toronto, ON, Canada.
[Agarwal, Arnav] Univ Toronto, Toronto, ON, Canada.
[Agarwal, Arnav] McMaster Univ, Hamilton, ON, Canada.
[Agrawal, Anurag] CSIR Inst Genom & Integrat Biol, Delhi, India.
[Agrawal, Anurag] Baylor Coll Med, Dept Internal Med, Houston, TX 77030 USA.
[Kiadaliri, Aliasghar Ahmad] Lund Univ, Clin Epidemiol Unit, Dept Clin Sci Lund, Orthoped, Lund, Sweden.
[Kiadaliri, Aliasghar Ahmad] Kerman Univ Med Sci, Inst Futures Studies Hlth, Hlth Serv Management Res Ctr, Kerman, Iran.
[Ajala, Oluremi N.] Univ Pittsburgh, Med Ctr, Mckeesport, PA USA.
[Akinyemiju, Tomi F.] Univ Alabama Birmingham, Dept Epidemiol, Birmingham, AL USA.
[Schwebel, David C.; Singh, Jasvinder A.] Univ Alabama Birmingham, Birmingham, AL USA.
[Al-Aly, Ziyad] Washington Univ, St Louis, MO USA.
[Alam, Noore K. M.] Queensland Hlth, Herston, Qld, Australia.
[Aldhahri, Saleh Fahed; Altirkawi, Khalid A.] King Saud Univ, Riyadh, Saudi Arabia.
[Aldhahri, Saleh Fahed; Terkawi, Abdullah Sulieman] King Fahad Med City, Dept Anesthesiol, Riyadh, Saudi Arabia.
[Aldhahri, Saleh Fahed] King Fahad Med City, Riyadh, Saudi Arabia.
[Aldridge, Robert William] UCL, Ctr Publ Hlth Data Sci, Inst Hlth Informat, London, England.
[Tillmann, Taavi] UCL, Dept Epidemiol & Publ Hlth, London, England.
[Alemu, Zewdie Aderaw; Tegegne, Teketo Kassaw] Debre Markos Univ, Debre Markos, Ethiopia.
[Alkerwi, Ala'a] Luxembourg Inst Hlth LIH, Strassen, Luxembourg.
[Alla, Francois; Guillemin, Francis] Univ Lorraine, Sch Publ Hlth, Nancy, France.
[Allebeck, Peter; Rabiee, Rynaz H. S.] Karolinska Inst, Dept Publ Hlth Sci, Stockholm, Sweden.
[Fereshtehnejad, Seyed-Mohammad] Karolinska Inst, Dept Neurobiol, Care Sci & Soc NVS, Stockholm, Sweden.
[Kivipelto, Miia] Karolinska Inst, Aging Res Ctr, Stockholm, Sweden.
[Weiderpass, Elisabete] Karolinska Inst, Dept Med Epidemiol & Biostat, Stockholm, Sweden.
[Havmoeller, Rasmus; Sindi, Shireen] Karolinska Inst, Stockholm, Sweden.
[Alsharif, Ubai] Charite, Berlin, Germany.
[Alvarez Martin, Elena] Govt Delegat Natl Plan Drugs, Minist Hlth, Spanish Observ Drugs, Social Policy & Equal, Madrid, Spain.
[Alvis-Guzman, Nelson] Univ Cartagena, Cartagena De Indias, Colombia.
[Amare, Azmeraw T.; Melaku, Yohannes Adama] Univ Adelaide, Sch Med, Adelaide, SA, Australia.
[Ciobanu, Liliana G.] Univ Adelaide, Adelaide, SA, Australia.
[Amare, Azmeraw T.] Bahir Dar Univ, Coll Med & Hlth Sci, Bahir Dar, Ethiopia.
[Taye, Belaynew Wasie] Bahir Dar Univ, Bahir Dar, Ethiopia.
[Amberbir, Alemayehu] Dignitas Int, Zomba, Malawi.
[Amegah, Adeladza Kofi] Univ Cape Coast, Cape Coast, Ghana.
[Amini, Heresh] Kurdistan Univ Med Sci, Environm Hlth Res Ctr, Sanandaj, Iran.
[Amini, Heresh; Fuerst, Thomas] Swiss Trop & Publ Hlth Inst, Dept Epidemiol & Publ Hlth, Basel, Switzerland.
[Karema, Corine Kakizi] Swiss Trop & Publ Hlth Inst, Basel, Switzerland.
[Ammar, Walid] Minist Publ Hlth, Beirut, Lebanon.
[Amrock, Stephen Marc] Oregon Hlth & Sci Univ, Portland, OR 97201 USA.
[Andersen, Hjalte H.] Aalborg Univ, Fac Med, Dept Hlth Sci & Technol, Ctr Sensory Motor Interact, Aalborg, Denmark.
[Antonio, Carl Abelardo T.] Univ Philippines Manila, Dept Hlth Policy & Adm, Coll Publ Hlth, Manila, Philippines.
[Aquino Faraon, Emerito Jose] Univ Philippines Manila, Coll Publ Hlth, Manila, Philippines.
[Arnlov, Johan; Larsson, Anders] Uppsala Univ, Dept Med Sci, Uppsala, Sweden.
[Arnlov, Johan] Dalarna Univ, Falun, Sweden.
Univ Manitoba, Winnipeg, MB, Canada.
[Asayesh, Hamid] Qom Univ Med Sci, Sch Paramed, Dept Emergency Med, Qom, Iran.
[Asghar, Rana Jawad] South Asian Publ Hlth Forum, Islamabad, Pakistan.
[Assadi, Reza] Mashhad Univ Med Sci, Mashhad, Iran.
[Atique, Suleman] Taipei Med Univ, Grad Inst Biomed Informat, Taipei, Taiwan.
[Avokpaho, Euripide Frinel G. Arthur] Inst Rech Clin Benin, Cotonou, Benin.
[Avokpaho, Euripide Frinel G. Arthur] Lab Etud & Rech Act Sante LERAS Afrique, Parakou, Benin.
[Awasthi, Ashish] Sanjay Gandhi Postgrad Inst Med Sci, Lucknow, Uttar Pradesh, India.
[Quintanilla, Beatriz Paulina Ayala] La Trobe Univ, Judith Lumley Ctr Mother Infant & Family Hlth Res, Melbourne, Vic, Australia.
[Quintanilla, Beatriz Paulina Ayala] Peruvian Natl Inst Hlth, Lima, Peru.
[Azzopardi, Peter] South Australian Hlth & Med Res Inst, Wardliparingga Aboriginal Res Unit, Adelaide, SA, Australia.
[Bacha, Umar] Univ Management & Technol, Sch Hlth Sci, Lahore, Pakistan.
[Badawi, Alaa] Publ Hlth Agcy Canada, Toronto, ON, Canada.
[Bahit, Maria C.] INECO Neurociencias, Rosario, Santa Fe, Argentina.
[Balakrishnan, Kalpana] Sri Ramachandra Univ, Dept Environm Hlth Engn, Madras, Tamil Nadu, India.
[Barac, Aleksandra] Univ Belgrade, Fac Med, Belgrade, Serbia.
[Barker-Collo, Suzanne L.] Univ Auckland, Sch Psychol, Auckland, New Zealand.
[del Pozo-Cruz, Borja] Univ Auckland, Auckland, New Zealand.
[Baernighausen, Till] Africa Hlth Res Inst, Mtubatuba, South Africa.
[Baernighausen, Till; Mohammed, Shafiu] Heidelberg Univ, Inst Publ Hlth, Heidelberg, Germany.
[Barregard, Lars] Univ Gothenburg, Dept Occupat & Environm Hlth, Gothenburg, Sweden.
[Petzold, Max] Univ Gothenburg, Hlth Metr Unit, Gothenburg, Sweden.
[Barrero, Lope H.] Pontificia Univ Javeriana, Sch Engn, Dept Ind Engn, Bogota, Colombia.
[Basu, Sanjay; Del Gobbo, Liana C.] Stanford Univ, Stanford, CA 94305 USA.
[Bazargan-Hejazi, Shahrzad] Charles R Drew Univ Med & Sci, Coll Med, 1621 E 120th St, Los Angeles, CA 90059 USA.
[Bazargan-Hejazi, Shahrzad] Univ Calif Los Angeles, David Geffen Sch Med, Los Angeles, CA 90095 USA.
[Bazargan-Hejazi, Shahrzad] Kermanshah Univ Med Sci, Kermanshah, Iran.
[Beardsley, Justin] Univ Oxford, Ho Chi Minh City, Vietnam.
[Bedi, Neeraj] Coll Publ Hlth & Trop Med, Jazan, Saudi Arabia.
[Beghi, Ettore] IRCCS Ist Ric Farmacol Mario Negri, Milan, Italy.
[Sheth, Kevin N.] Yale Univ, Sch Med, New Haven, CT USA.
[Bell, Michelle L.] Yale Univ, New Haven, CT USA.
[Bello, Aminu K.] Univ Alberta, Edmonton, AB, Canada.
[Santos, Itamar S.] Univ Sao Paulo, Dept Internal Med, Sao Paulo, Brazil.
[Bensenor, Isabela M.; Lotufo, Paulo A.] Univ Sao Paulo, Sao Paulo, Brazil.
[Berhane, Adugnaw] Debre Berhane Univ, Debre Berhan, Ethiopia.
[Wolfe, Charles D. A.] Kings Coll London, Div Hlth & Social Care Res, London, England.
[Bernabe, Eduardo] Kings Coll London, London, England.
Haramaya Univ, Coll Hlth & Med Sci, Harar, Ethiopia.
[Beyene, Addisu Shunu; Hassen, Tahir Ahmed; Mesfin, Yonatan Moges] Haramaya Univ, Harar, Ethiopia.
[Bhala, Neeraj] Queen Elizabeth Hosp Birmingham, Birmingham, W Midlands, England.
[Bhala, Neeraj] Univ Otago, Sch Med, Wellington, New Zealand.
[Bhansali, Anil] Postgrad Inst Med Educ & Res, Chandigarh, India.
[Biadgilign, Sibhatu] Independent Publ Hlth Consultants, Addis Ababa, Ethiopia.
[Bikbov, Boris] Acad VI Shumakov Fed Res Ctr Transplantol & Artif, Dept Nephrol Issues Transplanted Kidney, Moscow, Russia.
[Bjertness, Espen] Univ Oslo, Dept Community Med, Oslo, Norway.
[Htet, Aung Soe] Univ Oslo, Oslo, Norway.
[Boufous, Soufiane] Univ New South Wales, Transport & Rd Safety TARS Res, Kensington, NSW, Australia.
[Degenhardt, Louisa] Univ New South Wales, Natl Drug & Alcohol Res Ctr, Kensington, NSW, Australia.
[Resnikoff, Serge] Univ New South Wales, Brien Holden Vision Inst, Kensington, NSW, Australia.
[Calabria, Bianca] Univ New South Wales, Kensington, NSW, Australia.
[Bourne, Rupert R. A.] Anglia Ruskin Univ, Vis & Eye Res Unit, Cambridge, England.
[Brainin, Michael] Danube Univers Krems, Krems, Austria.
[Brazinova, Alexandra; Majdan, Marek] Trnava Univ, Dept Publ Hlth, Fac Hlth Sci & Social Work, Trnava, Slovakia.
[Brazinova, Alexandra] Int Neurotrauma Res Org, Vienna, Austria.
[Shen, Jiabin] Ohio State Univ, Coll Med, Columbus, OH 43210 USA.
[Breitborde, Nicholas J. K.] Ohio State Univ, Columbus, OH 43210 USA.
[Brenner, Hermann; Schoettker, Ben] German Canc Res Ctr, Heidelberg, Germany.
[Broday, David M.] Technion, Haifa, Israel.
[Brugha, Traolach S.] Univ Leicester, Leicester, Leics, England.
[Brunekreef, Bert; Kromhout, Hans] Univ Utrecht, Inst Risk Assessment Sci, Utrecht, Netherlands.
[Butt, Zahid A.] Al Shifa Trust Eye Hosp, Rawalpindi, Pakistan.
[van Donkelaar, Aaron] Dalhousie Univ, Dept Phys & Atmospher Sci, Halifax, NS, Canada.
[Cahill, Leah E.; Martin, Randall V.] Dalhousie Univ, Halifax, NS, Canada.
[Calabria, Bianca] Australian Natl Univ, Natl Ctr Epidemiol & Populat Hlth, Canberra, ACT, Australia.
[Cardenas, Rosario] Metropolitan Autonomous Univ, Mexico City, DF, Mexico.
[Carpenter, David] Univ Albany, Rensselaer, NY USA.
[Castaneda-Oquela, Carlos A.] Colombian Natl Hlth Observ, Inst Nacl Salud, Bogota, Colombia.
[Castaneda-Oquela, Carlos A.] Univ Nacl Colombia, Dept Publ Hlth, Epidemiol & Publ Hlth Evaluat Grp, Bogota, Colombia.
[Castillo Rivas, Jacqueline] Caja Costarricense Seguro Social, San Jose, Costa Rica.
[Castillo Rivas, Jacqueline] Univ Costa Rica, San Pedro, Montes De Oca, Costa Rica.
[Estanislao Castro, Ruben] Univ Diego Portales, Santiago, Chile.
[Catala-Lopez, Ferran] Univ Valencia, Dept Med, INCLIVA Hlth Res Inst, Valencia, Spain.
[Catala-Lopez, Ferran] CIBERSAM, Valencia, Spain.
[Catala-Lopez, Ferran] Ottawa Hosp, Res Inst, Clin Epidemiol Program, Ottawa, ON, Canada.
Natl Taiwan Univ, Coll Med, Sch Nursing, Taipei, Taiwan.
[Chiang, Peggy Pei-Chia] Gold Coast Hlth, Clin Governance Unit, Southport, Qld, Australia.
[Chibalabala, Mirriam] Crowd Watch Africa, Lusaka, Zambia.
[Chimed-Ochir, Odgerel] Univ Occupat & Environm Hlth, Dept Environm Epidemiol, Kitakyushu, Fukuoka, Japan.
[Jiang, Ying] Univ Occupat & Environm Hlth, Dept Hlth Dev, Inst Ind Ecol Sci, Kitakyushu, Fukuoka, Japan.
[Takahashi, Ken] Univ Occupat & Environm Hlth, Inst Ind Ecol Sci, Dept Environm Epidemiol, Kitakyushu, Fukuoka, Japan.
[Chisumpa, Vesper Hichilombwe; Mapoma, Chabila C.; Masiye, Felix] Univ Zambia, Lusaka, Zambia.
[Chisumpa, Vesper Hichilombwe] Univ Witwatersrand, Johannesburg, South Africa.
[Chitheer, Abdulaal A.] Minist Hlth, Baghdad, Iraq.
[Choi, Jee-Young Jasmine] Seoul Natl Univ, Med Lib, Seoul, South Korea.
[Christensen, Hanne] Bispebjerg Hosp, Copenhagen, Denmark.
[Christopher, Devasahayam Jesudas] Christian Med Coll & Hosp, Vellore, Tamil Nadu, India.
[Cooper, Leslie Trumbull] Mayo Clin, Jacksonville, FL 32224 USA.
Mario Negri Inst Pharmacol Res, Milan, Italy.
[Crump, John A.] Univ Otago, Ctr Int Hlth, Dunedin Sch Med, Dunedin, New Zealand.
[Poulton, Richie G.] Univ Otago, Dunedin, New Zealand.
[Damasceno, Albertino] Eduardo Mondlane Univ, Fac Med, Maputo, Mozambique.
[Dargan, Paul I.] Guys & St Thomas NHS Fdn Trust, London, England.
[das Neves, Jose] Univ Porto, Inst Invest & Inovacao Saude i3S, Oporto, Portugal.
[das Neves, Jose] Univ Porto, INEB Inst Engn Biomed, Oporto, Portugal.
[Davis, Adrian C.; Newton, John N.; Steel, Nicholas] Publ Hlth England, London, England.
[Davletov, Kairat] Kazakh Natl Med Univ, Sch Publ Hlth, Alma Ata, Kazakhstan.
[De Leo, Diego] Griffith Univ, Brisbane, Qld, Australia.
[Dellavalle, Robert P.] Univ Colorado, Sch Med, Aurora, CO USA.
[Dellavalle, Robert P.] Colorado Sch Publ Hlth, Aurora, CO USA.
[Deribew, Amare] KEMRI Wellcome Trust Res Programme, Kilifi, Kenya.
[Des Jarlais, Don C.] Mt Sinai Beth Israel, New York, NY USA.
[Des Jarlais, Don C.] Icahn Sch Med Mt Sinai, New York, NY 10029 USA.
[Dharmaratne, Samath D.] Univ Peradeniya, Fac Med, Dept Community Med, Peradeniya, Sri Lanka.
[Jeemon, Panniyammakal] Publ Hlth Fdn India, Ctr Control Chron Condit, Gurgaon, India.
[Dhillon, Preet K.; Lal, Dharmesh Kumar; Zodpey, Sanjay] Publ Hlth Fdn India, Gurgaon, India.
[Diaz-Tome, Cesar] Hosp Santa Creu & Sant Pau, Barcelona, Spain.
[Dorsey, E. Ray] Univ Rochester, Med Ctr, Rochester, NY 14642 USA.
[Doyle, Kerrie E.] RMIT Univ, Bundoora, Vic, Australia.
[Dubey, Manisha; Rahman, Mohammad Hifz Ur; Ram, Usha; Singh, Abhishek; Yadav, Ajit Kumar] Int Inst Populat Sci, Bombay, Maharashtra, India.
[Duncan, Bruce Bartholow; Kieling, Christian; Schmidt, Maria Ines] Univ Fed Rio Grande do Sul, Porto Alegre, RS, Brazil.
[Duncan, Bruce Bartholow] Univ Nouth Carolina, Chapel Hill, NC USA.
[Elyazar, Iqbal] Eijkman Oxford Clin Res Unit, Jakarta, Indonesia.
[Endries, Aman Yesuf] Arba Minch Univ, Arba Minch, Ethiopia.
[Ermakov, Sergey Petrovich] Russian Acad Sci, Inst Social & Econ Studies Populat, Moscow, Russia.
[Ermakov, Sergey Petrovich] Minist Hlth Russian Federat, Fed Res Inst Hlth Org & Informat, Moscow, Russia.
[Eshrati, Babak] Minist Hlth & Med Educ, Tehran, Iran.
[Eshrati, Babak] Arak Univ Med Sci, Arak, Iran.
[Farzadfar, Farshad; Kasaeian, Amir; Parsaeian, Mahboubeh] Univ Tehran Med Sci, Noncommunicable Dis Res Ctr, Tehran, Iran.
[Esteghamati, Alireza; Hafezi-Nejad, Nima; Sheikhbahaei, Sara] Univ Tehran Med Sci, Endocrinol & Metab Populat Sci Inst, Tehran, Iran.
[Fahimi, Saman; Malekzadeh, Reza; Roshandel, Gholamreza; Sepanlou, Sadaf G.] Univ Tehran Med Sci, Digest Dis Res Inst, Tehran, Iran.
[Hassanvand, Mohammad Sadegh] Univ Tehran Med Sci, Ctr Air Pollut Res, Inst Environm Res, Tehran, Iran.
[Heydarpour, Pouria] Univ Tehran Med Sci, Multiple Sclerosis Res Ctr, Neurosci Inst, Tehran, Iran.
[Kasaeian, Amir] Univ Tehran Med Sci, Hematol Oncol & Stem Cell Transplantat Res Ctr, Tehran, Iran.
[Parsaeian, Mahboubeh] Univ Tehran Med Sci, Dept Epidemiol & Biostat, Sch Publ Hlth, Tehran, Iran.
[Rahimi-Movaghar, Vafa] Univ Tehran Med Sci, Sina Trauma & Surg Res Ctr, Tehran, Iran.
[Yaseri, Mehdi] Univ Tehran Med Sci, Tehran, Iran.
[Aquino Faraon, Emerito Jose] Dept Hlth, Manila, Philippines.
[Farid, Talha A.; Khan, Abdur Rahman] Univ Louisville, Louisville, KY USA.
[Sofia E Sa Farinha, Carla] DGS Directorate Gen Hlth, Lisbon, Portugal.
[Sofia E Sa Farinha, Carla] Univ Aberta, Lisbon, Portugal.
[Faro, Andre] Univ Fed Sergipe, Aracaju, Brazil.
[Farvid, Maryam S.] Massachusetts Gen Hosp, Mongan Inst Hlth Policy, Harvard MGH Ctr Genom Vulnerable Populat & Hlth D, Boston, MA 02114 USA.
[Feigin, Valery L.] Auckland Univ Technol, Natl Inst Stroke & Appl Neurosci, Auckland, New Zealand.
[Fernandes, Jefferson G.] German Hosp Oswaldo Cruz, Inst Educ & Sci, Sao Paulo, Brazil.
[Fischer, Florian] Univ Bielefeld, Bielefeld, Germany.
[Foigt, Nataliya] Acad Med Sci, Inst Gerontol, Kiev, Ukraine.
[Shiue, Ivy] Univ Edinburgh, Alzheimer Scotland Dementia Res Ctr, Edinburgh, Midlothian, Scotland.
[Fowkes, F. Gerry R.] Univ Edinburgh, Edinburgh, Midlothian, Scotland.
[Franklin, Richard C.] James Cook Univ, Townsville, Qld, Australia.
[Garcia-Basteiro, Alberto L.] Manhica Hlth Res Ctr, Manhica, Mozambique.
[Garcia-Basteiro, Alberto L.] Barcelona Inst Global Hlth, Barcelona, Spain.
[Gebremedhin, Amanuel Tesfay] Univ Munich, Munich, Germany.
[Geleijnse, Johanna M.] Wageningen Univ, Div Human Nutr, Wageningen, Netherlands.
[Jibat, Tariku] Wageningen Univ, Wageningen, Netherlands.
[Gessner, Bradford D.] Agence Med Prevent, Paris, France.
[Tefera, Worku Mekonnen] Univ Addis Ababa, Coll Hlth Sci, Sch Publ Hlth, Addis Ababa, Ethiopia.
[Giref, Ababi Zergaw; Haile, Demewoz; Jibat, Tariku; Manamo, Wondimu Ayele Ayele] Univ Addis Ababa, Addis Ababa, Ethiopia.
[Giroud, Maurice] Univ Hosp Dijon, Dijon, France.
Haramaya Univ, Coll Hlth & Med Sci, Dire Dawa, Ethiopia.
[Gishu, Melkamu Dedefo; Tura, Abera Kenay] Haramaya Univ, Dire Dawa, Ethiopia.
[Gishu, Melkamu Dedefo] Kersa Hlth & Demog Surveillance Syst, Harar, Ethiopia.
[Martinez-Raga, Jose] Univ Valencia, Univ Hosp Doctor Peset, Valencia, Spain.
[Carmen Gomez-Cabrera, Mari] Univ Valencia, Valencia, Spain.
[Carmen Gomez-Cabrera, Mari] INCLIVA Biomed Res Inst, Valencia, Spain.
[Gona, Philimon] Univ Massachusetts, Boston, MA 02125 USA.
[Goodridge, Amador] Inst Invest Cient & Servicios Alta Tecnol INDICAS, Ciudad Del Saber, Panama.
[Gopalani, Sameer Vali] Govt Federated States Micronesia, Dept Hlth & Social Affairs, Palikir, Micronesia.
[Goto, Atsushi] Natl Canc Ctr, Div Epidemiol, Ctr Publ Hlth Sci, Tokyo, Japan.
[Inoue, Manami] Natl Canc Ctr, Tokyo, Japan.
[Gugnani, Harish Chander] St James Sch Med, Dept Microbiol, The Quarter, Anguilla, Scotland.
[Gugnani, Harish Chander] St James Sch Med, Dept Epidemiol & Biostat, The Quarter, Anguilla, Scotland.
West Virginia Bur Publ Hlth, Charleston, WV USA.
Eternal Heart Care Ctr & Res Inst, Jaipur, Rajasthan, India.
[Gutierrez, Reyna A.; Orozco, Ricardo] Natl Inst Psychiat Ramon Fuente, Mexico City, DF, Mexico.
[Haagsma, Juanita A.] Univ Med Ctr, Erasmus MC, Dept Publ Hlth, Rotterdam, Netherlands.
[Hailu, Gessessew Bugssa] Kilte Awlaelo Hlth & Demog Surveillance Syst, Mekelle, Ethiopia.
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[Maria Haro, Josep] Parc Sanitari Sant Joan Deu CIBERSAM, St Boi De Llobregat, Barcelona, Spain.
[Maria Haro, Josep] Univ Barcelona, Barcelona, Spain.
[Francisco Hernandez-Llanes, Norberto] Comis Nacl Adicc, Mexico City, DF, Mexico.
[Hoek, Hans W.] Univ Groningen, Univ Med Ctr Groningen, Dept Psychiat, Groningen, Netherlands.
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[Jacobs, Troy A.] HIDN, USAID Global Hlth Bur, MCH Div, Washington, DC USA.
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[Jansen, Henrica A. F. M.] UNFPA Asia & Pacific Reg Off, Bangkok, Thailand.
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[Jeemon, Panniyammakal] Ctr Chron Dis Control, New Delhi, India.
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[Jha, Vivekanand] George Inst Global Hlth India, New Delhi, India.
[Jonas, Jost B.] Heidelberg Univ, Med Fac Mannheim, Dept Ophthalmol, Mannheim, Germany.
[Kabir, Zubair] Univ Coll Cork, Cork, Ireland.
[Kalkonde, Yogeshwar] Soc Educ Act & Res Community Hlth, Gadchiroli, India.
[Kamal, Ritul] CSIR Indian Inst Toxicol Res, Lucknow, Uttar Pradesh, India.
[She, Jun] Fudan Univ, Dept Pulm Med, Zhongshan Hosp, Shanghai, Peoples R China.
[Kan, Haidong] Fudan Univ, Shanghai, Peoples R China.
[Karch, Andre] Helmholtz Ctr Infect Res, Epidemiol & Stat Methods Res Grp, Braunschweig, Germany.
[Karch, Andre] German Ctr Infect Res, Hannover Braunschweig Site, Braunschweig, Germany.
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[Keren, Andre] Assuta Hosp, Assuta Hashalom, Tel Aviv, Israel.
[Khader, Yousef Saleh] Jordan Univ Sci & Technol, Irbid, Jordan.
[Khan, Ejaz Ahmad] Hlth Serv Acad, Islamabad, Pakistan.
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[Khang, Young-Ho] Seoul Natl Univ, Coll Med, Seoul, South Korea.
[Won, Sungho] Seoul Natl Univ, Grad Sch Publ Hlth, Seoul, South Korea.
[Khera, Sahil] New York Med Coll, Valhalla, NY 10595 USA.
[Khoja, Tawfik Ahmed Muthafer] Execut Board Hlth Ministers Council Cooperat Coun, Riyadh, Saudi Arabia.
[Khubchandani, Jagdish] Ball State Univ, Muncie, IN 47306 USA.
[Kieling, Christian] Hosp Clin Porto Alegre, Porto Alegre, RS, Brazil.
Korea Hlth Ind Dev Inst, Cheongju, South Korea.
[Kim, Daniel] Northeastern Univ, Dept Hlth Sci, Boston, MA 02115 USA.
[Kimokoti, Ruth W.] Simmons Coll, Boston, MA 02115 USA.
[Kokubo, Yoshihiro] Natl Cerebral & Cardiovasc Ctr, Dept Prevent Cardiol, Suita, Osaka, Japan.
[Koul, Parvaiz A.] Sherikashmir Inst Med Sci, Srinagar, Jammu & Kashmir, India.
[Koyanagi, Ai] Parc Sanitari St Joan Deu CIBERSAM, Res & Dev Unit, Barcelona, Spain.
[Kravchenko, Michael; Varakin, Yuri Y.] Res Ctr Neurol, Moscow, Russia.
[Defo, Barthelemy Kuate] Univ Montreal, Dept Demog, Montreal, PQ, Canada.
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[Kuchenbecker, Ricardo S.] Univ Fed Rio Grande do Sul, Graduat Studies Epidemiol, Porto Alegre, RS, Brazil.
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[Meretoja, Tuomo J.] Univ Helsinki, Helsinki, Finland.
[Lan, Qing] NCI, Rockville, MD USA.
[Latif, Asma Abdul] Women Univ, Lahore Coll, Dept Zool, Lahore, Pakistan.
[Beatriz Lawrynowicz, Alicia Elena] Inst Nacl Epidemiol Dr Juan H Jara, Mar Del Plata, Buenos Aires, Argentina.
[Leasher, Janet L.] Nova Southeastern Univ, Coll Optometry, Ft Lauderdale, FL 33314 USA.
[Levi, Miriam] Tuscany Reg Ctr Occupat Injuries & Dis, Florence, Italy.
[Li, Xiaohong] Natl Ctr Birth Defects Monitoring China, Chengdu, Peoples R China.
[Liang, Juan] Sichuan Univ, West China Univ Hosp 2, Natl Off Maternal & Child Hlth Surveillance, Chengdu, Peoples R China.
[Lloyd, Belinda K.] Monash Univ, Eastern Hlth Clin Sch, Fitzroy, Vic, Australia.
[Lloyd, Belinda K.] Eastern Hlth, Turning Point, Melbourne, Vic, Australia.
[Logroscino, Giancarlo] Univ Bari, Bari, Italy.
[Lunevicius, Raimundas] Aintree Univ, Hosp Natl Hlth Serv Fdn Trust, Liverpool, Merseyside, England.
[Lunevicius, Raimundas] Univ Liverpool, Sch Med, Liverpool, Merseyside, England.
[Pope, Daniel] Univ Liverpool, Dept Publ Hlth & Policy, Liverpool, Merseyside, England.
[Mahdavi, Mandi] Social Secur Org Res Inst, Tehran, Iran.
[Mahdavi, Mandi] Erasmus Univ, Inst Hlth Policy & Management, Rotterdam, Netherlands.
[Malta, Deborah Carvalho] Univ Fed Minas Gerais, Belo Horizonte, MG, Brazil.
[Marcenes, Wagner] Kings Coll London, Inst Dent, Div Populat & Patient Hlth, London, England.
[Martinez-Raga, Jose] CEU Cardenal Herrera Univ, Moncada, Valencia, Spain.
[Matsushita, Kunihiro; Nachega, Jean B.] Johns Hopkins Univ, Bloomberg Sch Publ Hlth, Baltimore, MD USA.
[Bach Xuan Tran] Johns Hopkins Univ, Baltimore, MD USA.
[Meaney, Peter A.] Univ Penn, Perelman Sch Med, Philadelphia, PA 19104 USA.
[Meaney, Peter A.] Childrens Hosp Philadelphia, Philadelphia, PA 19104 USA.
[Mehari, Alem] Howard Univ, Coll Med, Washington, DC 20059 USA.
[Mekonnen, Alemayehu B.; Tedla, Bemnet Amare] Univ Gondar, Gondar, Ethiopia.
[Memish, Ziad A.] Saudi Minist Hlth, Riyadh, Saudi Arabia.
[Memish, Ziad A.] Alfaisal Univ, Coll Med, Riyadh, Saudi Arabia.
[Mendoza, Walter] United Nations Populat Fund, Lima, Peru.
[Mensink, Gert B. M.] Robert Koch Inst, Berlin, Germany.
[Meretoja, Atte] Helsinki Univ Hosp, Dept Neurol, Helsinki, Finland.
[Meretoja, Tuomo J.] Helsinki Univ Hosp, Ctr Comprehens Canc, Breast Surg Unit, Helsinki, Finland.
[Mhimbira, Francis Apolinary] Ifakara Hlth Inst, Bagamoyo, Tanzania.
[Miller, Ted R.] Pacific Inst Res & Evaluat, Calverton, MD USA.
[Miller, Ted R.] Curtin Univ, Ctr Populat Hlth, Perth, WA, Australia.
[Mills, Edward J.] Univ Ottawa, Ottawa, ON, Canada.
[Mohammadi, Alireza] Baqiyatallah Univ Med Sci, Neurosci Res Ctr, Tehran, Iran.
[Mohammed, Shafiu] Ahmadu Bello Univ, Hlth Syst & Policy Res Unit, Zaria, Nigeria.
[Mola, Glen Liddell D.] Univ Papua New Guinea, Boroko, Papua N Guinea.
[Monasta, Lorenzo; Montico, Marcella; Ronfani, Luca] IRCCS Burlo Garofolo, Inst Maternal & Child Hlth, Trieste, Italy.
[Moradi-Lakeh, Maziar] Iran Univ Med Sci, Dept Community Med, Gastrointestinal & Liver Dis Res Ctr, Prevent Med & Publ Hlth Res Ctr, Tehran, Iran.
[Morawska, Lidia] Queensland Univ Technol, Int Lab Air Qual & Hlth, Brisbane, Qld, Australia.
[Norman, Rosana E.] Queensland Univ Technol, Inst Hlth & Biomed Innovat, Brisbane, Qld, Australia.
[Mori, Rintaro] Natl Ctr Child Hlth & Dev, Tokyo, Japan.
[Mozaffarian, Dariush] Tufts Univ, Friedman Sch Nutr Sci & Policy, Boston, MA 02111 USA.
[Shi, Peilin] Tufts Univ, Boston, MA 02111 USA.
[Werdecker, Andrea] Fed Inst Populat Res, Competence Ctr Mortal Follow Up German Natl Cohor, Wiesbaden, Germany.
[Mueller, Ulrich O.; Westerman, Ronny] Fed Inst Populat Res, Wiesbaden, Germany.
[Murthy, Gudlavalleti Venkata Satyanarayana] Publ Hlth Fdn India, Indian Inst Publ Hlth, Gurgaon, India.
[Dhillon, Preet K.; Lal, Dharmesh Kumar; Zodpey, Sanjay] Publ Hlth Fdn India, Gurgaon, India.
[Nachega, Jean B.] Univ Pittsburgh, Grad Sch Publ Hlth, Pittsburgh, PA USA.
[Caicedo, Angel J. Paternina] Univ Pittsburgh, Publ Hlth Dynam Lab, Pittsburgh, PA USA.
[Parry, Charles D.] Univ Stellenbosch, Dept Psychiat, Cape Town, South Africa.
[Nachega, Jean B.; Seedat, Soraya; Wiysonge, Charles Shey] Univ Stellenbosch, Cape Town, South Africa.
[Naheed, Aliya] Int Ctr Diarrhoeal Dis Res, Bangladesh Icddr B, Dhaka, Bangladesh.
[Nangia, Vinay] Suraj Eye Inst, Nagpur, Maharashtra, India.
[Nassiri, Nariman] Wayne State Univ, Sch Med, Detroit, MI USA.
[Quyen Le Nguyen] Duy Tan Univ, Inst Global Hlth Innovat, Da Nang, Vietnam.
[Pete, Patrick Martial Nkamedjie] Inst Res Socioecon Dev & Commun, Yaounde, Cameroon.
[Vollset, Stein Emil] Univ Bergen, Dept Global Publ Hlth & Primary Care, Bergen, Norway.
[Norheim, Ole F.] Univ Bergen, Bergen, Norway.
[Norrving, Bo] Skane Univ Hosp, Dept Clin Sci Lund, Dept Clin Sci, Lund, Sweden.
[Nyakarahuka, Luke] Makerere Univ, Kampala, Uganda.
[Obermeyer, Carla Makhlouf] Amer Univ Beirut, Fac Hlth Sci, Ctr Res Populat & Hlth, Beirut, Lebanon.
[Ogbo, Felix Akpojene] Univ Western Sydney, Ctr Hlth Res, Sydney, NSW, Australia.
Kyung Hee Univ, Sch Med, Dept Prevent Med, Seoul, South Korea.
[Oladimeji, Olanrewaju] Human Sci Res Council, Durban, South Africa.
[Oladimeji, Olanrewaju; Sartorius, Benn] Univ KwaZulu Natal, Durban, South Africa.
Univ Autonoma Chile, Talca, Chile.
[Olusanya, Bolajoko Olubukunola; Olusanya, Jacob Olusegun] Ctr Hlth Start Initiat, Lagos, Nigeria.
[Opio, John Nelson] Lira Municipal Council, Lira Dist Local Govt, Lira, Uganda.
[Oren, Eyal] Univ Arizona, Tucson, AZ USA.
[Ortiz, Alberto] II S Fdn Jimenez Diaz UAM, Madrid, Spain.
[Ota, Erika] St Lukes Int Univ, Tokyo, Japan.
[Mahesh, P. A.] JSS Univ, JSS Med Coll, Mysore, Karnataka, India.
Kosin Univ, Coll Med, Dept Med Human & Social Med, Busan, South Korea.
[Patel, Tejas] Mt Sinai Hlth Syst, New York, NY USA.
[Caicedo, Angel J. Paternina] Univ Cartagena, Cartagena, Colombia.
[Patil, Snehal T.] Deemed Univ, Krishan Inst Med Sci, Sch Dent Sci, Karad, India.
[Patten, Scott B.] Univ Calgary, Dept Community Hlth Sci, Calgary, AB, Canada.
[Wang, JianLi] Univ Calgary, Calgary, AB, Canada.
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[Perico, Norberto; Remuzzi, Giuseppe] IRCCS Ist Ric Farmacol Mario Negri, Bergamo, Italy.
[Pesudovs, Konrad] Flinders Univ S Australia, Adelaide, SA, Australia.
[Petzold, Max] Univ Witwatersrand, Johannesburg, South Africa.
[Phillips, Michael Robert] Shanghai Jiao Tong Univ, Sch Med, Shanghai, Peoples R China.
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[Phillips, Michael Robert] Emory Univ, Atlanta, GA 30322 USA.
[Pillay, Julian David] Durban Univ Technol, Durban, South Africa.
[Plass, Dietrich] German Environm Agcy, Exposure Assessment & Environm Hlth Indicators, Berlin, Germany.
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[Polinder, Suzanne] Erasmus Univ, Med Ctr, Dept Publ Hlth, Rotterdam, Netherlands.
[Pond, Constance D.] Univ Newcastle, Callaghan, NSW, Australia.
[Pope, C. Arden] Brigham Young Univ, Provo, UT 84602 USA.
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[Prasad, Noela M.] Ctr Eye Res Australia, Melbourne, Vic, Australia.
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[Rafay, Anwar; Rana, Saleem M.] Contech Sch Publ Hlth, Lahore, Pakistan.
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[Rahman, Sajjad Ur] Hamad Med Corp, Doha, Qatar.
[Rai, Rajesh Kumar] Soc Hlth & Demog Surveillance, Suri, India.
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[Rana, Saleem M.] Contech Int Hlth Consultants, Lahore, Pakistan.
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[Refaat, Amany H.] Suez Canal Univ, Ismailia, Egypt.
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[Remuzzi, Giuseppe] Azienda Osped Papa Giovanni XXIII, Bergamo, Italy.
[Remuzzi, Giuseppe] Univ Milan, Dept Biomed & Clin Sci L Sacco, Milan, Italy.
[Ribeiro, Antonio L.] Univ Fed Minas Gerais, Hosp Clin, Belo Horizonte, MG, Brazil.
[Rodriguez, Anna] Lincoln Univ, Sch Psychol, Lincoln, England.
[Rojas-Rueda, David] Inst Salud Global Barcelona, Barcelona, Spain.
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[Saleh, Muhammad Muhammad] Dev Res & Projects Ctr, Abuja, Nigeria.
[Sanabria, Juan R.] Marshall Univ, J Edwards Sch Med, Huntington, WV USA.
Case Western Reserve Univ, Cleveland, OH 44106 USA.
[Dolores Sanchez-Nino, Maria] II S Fdn Jimenez Diaz, Madrid, Spain.
[Sarmiento-Suarez, Rodrigo] Univ Ciencias Aplicadas & Ambient, Bogota, Colombia.
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[Schmidhuber, Josef] Food & Agr Org, Global Perspect Studies Unit, Rome, Italy.
[Schneider, Ione J. C.] Univ Fed Santa Catarina, Florianopolis, SC, Brazil.
[Schoettker, Ben] FOM Univ, Inst Hlth Care & Social Sci, Essen, Germany.
[Schutte, Aletta E.] North West Univ, Hypertens Africa Res Team HART, Potchefstroom, South Africa.
[Parry, Charles D.] South African Med Res Council, Alcohol Tobacco & Other Drug Res Unit, Potchefstroom, South Africa.
[Schutte, Aletta E.] South African Med Res Council, Potchefstroom, South Africa.
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[Shaikh, Masood Ali] Tufts Med Ctr, Boston, MA USA.
[Shaikh, Masood Ali] Independent Consultant, Karachi, Pakistan.
[Sharma, Rajesh] Indian Inst Technol Ropar, Rupnagar, India.
[Shen, Jiabin] Nationwide Childrens Hosp, Res Inst, Columbus, OH USA.
[Shigematsu, Mika] Natl Inst Infect Dis, Tokyo, Japan.
[Shigematsu, Mika] Sandia Natl Labs, Albuquerque, NM USA.
Korea Univ, Dept Publ Hlth Sci, Grad Sch, Seoul, South Korea.
Korea Univ, Dept Prevent Med, Coll Med, Seoul, South Korea.
[Shishani, Kawkab] Washington State Univ, Spokane, WA USA.
[Shiue, Ivy] Northumbria Univ, Fac Hlth & Life Sci, Newcastle Upon Tyne, Tyne & Wear, England.
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[Silverberg, Jonathan I.] Northwestern Univ, Feinberg Sch Med, Chicago, IL 60611 USA.
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[Singh, Prashant Kumar] Inst Human Dev, New Delhi, India.
[Soneji, Samir] Dartmouth Coll, Hanover, NH 03755 USA.
[Sposato, Luciano A.] Western Univ, Dept Clin Neurol Sci, London, ON, Canada.
[Sreeramareddy, Chandrashekhar T.] Int Med Univ, Dept Community Med, Kuala Lumpur, Malaysia.
[Stathopoulou, Vasiliki] Attikon Univ Hosp, Athens, Greece.
[Steckling, Nadine] Univ Hosp Munich, Inst & Outpatient Clin Occupat Social & Environm, Munich, Germany.
[Steel, Nicholas] Univ East Anglia, Norwich, Norfolk, England.
[Stein, Dan J.] South African Med Res Council Unit Anxiety & Stre, Cape Town, South Africa.
[Stranges, Saverio] Luxembourg Inst Hlth, Strassen, Luxembourg.
[Stroumpoulis, Konstantinos] Alexandra Gen Hosp Athens, Athens, Greece.
[Stroumpoulis, Konstantinos] Ctr Hosp Publ Cotentin, Cherbourg, France.
[Sunguya, Bruno F.] Muhimbili Univ Hlth & Allied Sci, Dar Es Salaam, Tanzania.
[Swaminathan, Soumya] Indian Council Med Res, New Delhi, India.
[Sykes, Bryan L.] Univ Calif Irvine, Dept Criminol, Irvine, CA USA.
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[Tabares-Seisdedos, Rafael] Univ Valencia, Dept Med, INCLIVA Hlth Res Inst, Valencia, Spain.
[Tabares-Seisdedos, Rafael] CIBERSAM, Valencia, Spain.
[Talongwa, Roberto Tchio] MINSANTE, Minist Hlth, Yaounde, Cameroon.
[Tanne, David] Chaim Sheba Med Ctr, Tel Hashomer, Israel.
[Tanne, David] Tel Aviv Univ, Tel Aviv, Israel.
[Tedla, Bemnet Amare] James Cook Univ, Cairns, Qld, Australia.
[Terkawi, Abdullah Sulieman] Univ Virginia, Dept Anesthesiol, Charlottesville, VA USA.
[Terkawi, Abdullah Sulieman] Cleveland Clin, Outcomes Res Consortium, Cleveland, OH 44106 USA.
[Tuzcu, Emin Murat] Cleveland Clin, Cleveland, OH 44106 USA.
[Thakur, J. S.] Post Grad Inst Med Educ & Res, Sch Publ Hlth, Chandigarh, India.
Univ Bath, Bath, Avon, England.
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[Thorne-Lyman, Andrew L.] WorldFish, George Town, Malaysia.
[Thrift, Amanda G.] Monash Univ, Sch Clin Sci Monash Hlth, Dept Med, Melbourne, Vic, Australia.
[Thurston, George D.] New York Univ, Sch Med, Nelson Inst Environm Med, Tuxedo Pk, NY USA.
[Tobe-Gai, Ruoyan] Natl Ctr Child Hlth & Dev, Tokyo, Japan.
[Topor-Madry, Roman] Jagiellonian Univ, Coll Med, Fac Hlth Sci, Inst Publ Hlth, Krakow, Poland.
[Topor-Madry, Roman] Wroclaw Med Univ, Fac Hlth Sci, Wroclaw, Poland.
[Topouzis, Fotis] Aristotle Univ Thessaloniki, Thessaloniki, Greece.
[Towbin, Jeffrey Allen] Le Bonheur Childrens Hosp, Memphis, TN USA.
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[Towbin, Jeffrey Allen] St Jude Childrens Res Hosp, 332 N Lauderdale St, Memphis, TN 38105 USA.
[Bach Xuan Tran] Hanoi Med Univ, Hanoi, Vietnam.
[Dimbuene, Zacharie Tsala] Univ Kinshasa, Fac Econ & Management, Dept Populat Sci & Dev, Kinshasa, Congo.
[Dimbuene, Zacharie Tsala] African Populat & Hlth Res Ctr, Nairobi, Kenya.
[Tsilimparis, Nikolaos] Univ Heart Ctr Hamburg, Hamburg, Germany.
[Tyrovolas, Stefanos] Univ Barcelona, CIBERSAM, Fundacio St Joan De Deu, Parc Sanitari Sant Joan De Deu, Barcelona, Spain.
[Ukwaja, Kingsley N.] Fed Teaching Hosp, Dept Internal Med, Abakaliki, Nigeria.
[Uneke, Chigozie Jesse] Ebonyi State Univ, Abakaliki, Nigeria.
[Uthman, Olalekan A.] Univ Warwick, Warwick Med Sch, Coventry, W Midlands, England.
[van Os, Jim] Maastricht Univ, Med Ctr, Maastricht, Netherlands.
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[Venketasubramanian, Narayanaswamy] Raffles Hosp, Raffles Neurosci Ctr, Singapore, Singapore.
[Violante, Francesco S.] Univ Bologna, Bologna, Italy.
[Wagner, Gregory R.] Natl Inst Occupat Safety & Hlth, Washington, DC USA.
[Waller, Stephen G.] Uniformed Serv Univ Hlth Sci, Bethesda, MD 20814 USA.
[Wang, Yanping] Natl Off Maternal & Child Hlth Surveillance, Chengdu, Peoples R China.
[Weichenthal, Scott] McGill Univ, Montreal, PQ, Canada.
[Weiderpass, Elisabete] Inst Populat Based Canc Res, Dept Res, Canc Registry Norway, Oslo, Norway.
[Weiderpass, Elisabete] Arctic Univ Norway, Univ Tromso, Fac Hlth Sci, Dept Community Med, Tromso, Norway.
[Weiderpass, Elisabete] Folkhalsan Res Ctr, Genet Epidemiol Grp, Helsinki, Finland.
[Weintraub, Robert G.] Royal Childrens Hosp, Melbourne, Vic, Australia.
[Westerman, Ronny] German Natl Cohort Consortium, Heidelberg, Germany.
[Wijeratne, Tissa] Western Hlth, Footscray, Vic, Australia.
Guys & St Thomas NHS Fdn Trust, Comprehens Biomed Res Ctr, Natl Inst Hlth Res, London, England.
Kings Coll London, London, England.
[Woolf, Anthony D.] Royal Cornwall Hosp, Truro, England.
[Wubshet, Mamo] St Pauls Hosp, Millennium Med Coll, Addis Ababa, Ethiopia.
[Xavier, Denis] St Johns Med Coll & Res Inst, Bangalore, Karnataka, India.
[Xu, Gelin] Nanjing Univ, Sch Med, Jinling Hosp, Dept Neurol, Nanjing, Jiangsu, Peoples R China.
[Yakob, Bereket] Univ KwaZulu Natal, Sch Nursing & Publ Hlth, Discipline Publ Hlth Med, Durban, South Africa.
[Yip, Paul] Univ Hong Kong, Social Work & Social Adm Dept, Hong Kong, Hong Kong, Peoples R China.
[Yip, Paul] Univ Hong Kong, Hong Kong Jockey Club Ctr Suicide Res & Prevent, Hong Kong, Hong Kong, Peoples R China.
[Yonemoto, Naohiro] Kyoto Univ, Sch Publ Hlth, Dept Biostat, Kyoto, Japan.
[Younis, Mustafa Z.] Jackson State Univ, Jackson, MS USA.
[Yu, Chuanhua] Wuhan Univ, Dept Epidemiol & Biostat, Sch Publ Hlth, Wuhan, Peoples R China.
[Yu, Chuanhua] Wuhan Univ, Global Hlth Inst, Wuhan, Peoples R China.
[Zaidi, Zoubida] Univ Hosp, Setif, Algeria.
[Zaki, Maysaa El Sayed] Mansoura Univ, Fac Med, Mansoura, Egypt.
[Zhu, Jun] Natl Off MCH Surveillance China, Chengdu, Peoples R China.
[Zuhlke, Liesl Joanna] Red Cross War Mem Childrens Hosp, Cape Town, South Africa.
RP Murray, CJL (reprint author), Inst Hlth Metr & Evaluat, Seattle, WA 98121 USA.
EM cjlm@uw.edu
RI Ribeiro, Antonio/C-2707-2009; Salomon, Joshua/D-3898-2009; Monasta,
Lorenzo/B-1388-2012; Hankey, Graeme /H-4968-2014; Kravchenko,
Michael/B-2596-2012; Patton, George/B-5246-2013; Malta,
Deborah/H-7880-2012; Varakin, Yuriy/C-8634-2012; Brenner,
Hermann/B-4627-2017; Martinez-Raga, Jose/B-6251-2017; Majdan,
Marek/K-5017-2012; Weiderpass, Elisabete/M-4029-2016; Davletov,
Kairat/S-1792-2016; Gishu, Melkamu Dedefo/C-3747-2017; Alsharif,
Ubai/C-6527-2017; Amini, Heresh/B-3076-2010; Lotufo, Paulo/A-9843-2008;
Karch, Andre/D-6973-2017; Patten, Scott/B-4434-2011; Scott,
James/D-5900-2012; Giussani, Giorgia/E-8057-2017; Abbas,
Kaja/E-6590-2017; Pereira, David/M-9286-2013;
OI Ribeiro, Antonio/0000-0002-2740-0042; Salomon,
Joshua/0000-0003-3929-5515; Monasta, Lorenzo/0000-0001-7774-548X;
Hankey, Graeme /0000-0002-6044-7328; Kravchenko,
Michael/0000-0001-5187-5518; Patton, George/0000-0001-5039-8326; Malta,
Deborah/0000-0002-8214-5734; Brenner, Hermann/0000-0002-6129-1572;
Martinez-Raga, Jose/0000-0002-2856-6562; Majdan,
Marek/0000-0001-8037-742X; Weiderpass, Elisabete/0000-0003-2237-0128;
Gishu, Melkamu Dedefo/0000-0002-3466-1232; Alsharif,
Ubai/0000-0002-4024-3950; Amini, Heresh/0000-0002-4825-1322; Lotufo,
Paulo/0000-0002-4856-8450; Karch, Andre/0000-0003-3014-8543; Patten,
Scott/0000-0001-9871-4041; Scott, James/0000-0002-0744-0688; Abbas,
Kaja/0000-0003-0563-1576; Pereira, David/0000-0003-0384-7592;
Sreeramareddy, Chandrashekhar/0000-0002-5693-7631; Miller,
Ted/0000-0002-0958-2639; Agrawal, Anurag/0000-0002-0340-5252; Kemp,
Andrew/0000-0003-1146-3791; Charlson, Fiona/0000-0003-2876-5040; das
Neves, Jose/0000-0002-2317-2759; Degenhardt, Louisa/0000-0002-8513-2218;
Awasthi, Ashish/0000-0002-9308-9782; Bisanzio,
Donal/0000-0002-7832-2291; Jacobsen, Kathryn/0000-0002-4198-6246;
Bernabe, Eduardo/0000-0002-1858-3713; Atique,
Suleman/0000-0002-5149-0703; Piel, Frederic B./0000-0001-8131-7728;
Altirkawi, Khalid/0000-0002-7331-4196; Hoek, Hans/0000-0001-6353-5465;
NORMAN, ROSANA/0000-0002-9742-1957; Xu, Gelin/0000-0002-6194-0341;
Al-Aly, Ziyad/0000-0002-2600-0434; assadi, reza/0000-0002-5016-2994;
Heydarpour, Pouria/0000-0001-5644-7555; Alkerwi,
Ala'a/0000-0002-7448-3936; Ahmad Kiadaliri,
Aliasghar/0000-0002-4254-9099; Kieling, Christian/0000-0001-7691-4149;
Javanbakht, Mehdi/0000-0002-8661-8439; Gething,
Peter/0000-0001-6759-5449; Husseini, Abdullatif/0000-0001-8767-5956;
Taylor, Hugh/0000-0002-9437-784X
FU Bill AMP; Melinda Gates Foundation
FX Bill & Melinda Gates Foundation.
NR 139
TC 18
Z9 18
U1 88
U2 88
PU ELSEVIER SCIENCE INC
PI NEW YORK
PA 360 PARK AVE SOUTH, NEW YORK, NY 10010-1710 USA
SN 0140-6736
EI 1474-547X
J9 LANCET
JI Lancet
PD OCT 8
PY 2016
VL 388
IS 10053
BP 1659
EP 1724
PG 66
WC Medicine, General & Internal
SC General & Internal Medicine
GA DY7BU
UT WOS:000385285000010
ER
PT J
AU Goldan, AH
Li, C
Pennycook, SJ
Schneider, J
Blom, A
Zhao, W
AF Goldan, A. H.
Li, C.
Pennycook, S. J.
Schneider, J.
Blom, A.
Zhao, W.
TI Molecular structure of vapor-deposited amorphous selenium
SO JOURNAL OF APPLIED PHYSICS
LA English
DT Article
ID CHALCOGENIDE GLASSES; DYNAMICS SIMULATION; LIQUID SELENIUM; RING;
RELAXATION; STATE; SPECTROSCOPY; TRANSITION; TELLURIUM; VISCOSITY
AB The structure of amorphous selenium is clouded with much uncertainty and contradictory results regarding the dominance of polymeric chains versus monomer rings. The analysis of the diffraction radial distribution functions are inconclusive because of the similarities between the crystalline allotropes of selenium in terms of the coordination number, bond length, bond angle, and dihedral angle. Here, we took a much different approach and probed the molecular symmetry of the thermodynamically unstable amorphous state via analysis of structural phase transformations. We verified the structure of the converted metastable and stable crystalline structures using scanning transmission electron microscopy. In addition, given that no experimental technique can tell us the exact three-dimensional atomic arrangements in glassy semiconductors, we performed molecular-dynamic simulations using a well-established empirical three-body interatomic potential. We developed a true vapor-deposited process for the deposition of selenium molecules onto a substrate using empirical molecular vapor compositions and densities. We prepared both vapor-deposited and melt-quenched samples and showed that the simulated radial distribution functions match very well to experiment. The combination of our experimental and molecular-dynamic analyses shows that the structures of vapor-and melt-quenched glassy/amorphous selenium are quite different, based primarily on rings and chains, respectively, reflecting the predominant structure of the parent phase in its thermodynamic equilibrium. Published by AIP Publishing.
C1 [Goldan, A. H.; Zhao, W.] SUNY Stony Brook, Sch Med, Dept Radiol, Stony Brook, NY 11794 USA.
[Li, C.] Oak Ridge Natl Lab, Div Mat Sci & Technol, Oak Ridge, TN 37831 USA.
[Pennycook, S. J.] Natl Univ Singapore, Dept Mat Sci & Engn, Singapore 117575, Singapore.
[Schneider, J.; Blom, A.] QuantumWise AS, Fruebjergvej 3,Postbox 4, DK-2100 Copenhagen, Denmark.
[Li, C.] Univ Vienna, Dept Lithospher Res, A-1090 Vienna, Austria.
RP Goldan, AH (reprint author), SUNY Stony Brook, Sch Med, Dept Radiol, Stony Brook, NY 11794 USA.
EM Amirhossein.Goldan@stonybrookmedicine.edu
OI Li, Chen/0000-0001-9839-6100
FU Stony Brook University; NIH [1 R01 CA148053, 1 R01 EB002655]; U.S.
Department of Energy (DOE) Office of Basic Energy Sciences (BES),
Materials Science and Engineering Division; ORNL's Center for Nanophase
Materials Sciences (CNMS); DOE-BES; U.S. Department of Energy, Office of
Basic Energy Sciences [DE-AC02-98CH10886]
FX This research was supported by Stony Brook University's Seed grant, NIH
(1 R01 CA148053 and 1 R01 EB002655), the U.S. Department of Energy (DOE)
Office of Basic Energy Sciences (BES), Materials Science and Engineering
Division (C.L., S.J.P), and through a user project supported by ORNL's
Center for Nanophase Materials Sciences (CNMS), which is also sponsored
by DOE-BES. Amorphous selenium films were deposited at Analogic
Corporation, Montreal, QC, Canada. Raman spectroscopy measurements were
carried out at the Center for Functional Nanomaterials, Brookhaven
National Laboratory, which is supported by the U.S. Department of
Energy, Office of Basic Energy Sciences, under Contract No.
DE-AC02-98CH10886.
NR 53
TC 0
Z9 0
U1 3
U2 3
PU AMER INST PHYSICS
PI MELVILLE
PA 1305 WALT WHITMAN RD, STE 300, MELVILLE, NY 11747-4501 USA
SN 0021-8979
EI 1089-7550
J9 J APPL PHYS
JI J. Appl. Phys.
PD OCT 7
PY 2016
VL 120
IS 13
AR 135101
DI 10.1063/1.4962315
PG 9
WC Physics, Applied
SC Physics
GA DZ8XE
UT WOS:000386155100025
ER
PT J
AU Jones, DR
Fensin, SJ
Dippo, O
Beal, RA
Livescu, V
Martinez, DT
Trujillo, CP
Florando, JN
Kumar, M
Gray, GT
AF Jones, D. R.
Fensin, S. J.
Dippo, O.
Beal, R. A.
Livescu, V.
Martinez, D. T.
Trujillo, C. P.
Florando, J. N.
Kumar, M.
Gray, G. T., III
TI Spall fracture in additive manufactured Ti-6Al-4V
SO JOURNAL OF APPLIED PHYSICS
LA English
DT Article
ID LASER-MELTED TI-6AL-4V; MICROSTRUCTURE
AB We present a study on the spall strength of additive manufactured (AM) Ti-6Al-4V. Samples were obtained from two pieces of selective laser melted (SLM, a powder bed fusion technique) Ti-6Al-4V such that the response to dynamic tensile loading could be investigated as a function of the orientation between the build layers and the loading direction. A sample of wrought bar-stock Ti6Al-4V was also tested to act as a baseline representing the traditionally manufactured material response. A single-stage light gas-gun was used to launch a thin flyer plate into the samples, generating a region of intense tensile stress on a plane normal to the impact direction. The rear free surface velocity time history of each sample was recorded with laser-based velocimetry to allow the spall strength to be calculated. The samples were also soft recovered to enable post-mortem characterization of the spall damage evolution. Results showed that when the tensile load was applied normal to the interfaces between the build layers caused by the SLM fabrication process the spall strength was drastically reduced, dropping to 60% of that of the wrought material. However, when loaded parallel to the AM build layer interfaces the spall strength was found to remain at 95% of the wrought control, suggesting that when loading normal to the AM layer interfaces, void nucleation is facilitated more readily due to weaknesses along these boundaries. Quasi-static testing of the same sample orientations revealed a much lower degree of anisotropy, demonstrating the importance of rate-dependent studies for damage evolution in AM materials. Published by AIP Publishing.
C1 [Jones, D. R.; Fensin, S. J.; Dippo, O.; Beal, R. A.; Livescu, V.; Martinez, D. T.; Trujillo, C. P.; Gray, G. T., III] Los Alamos Natl Lab, MST 8, Los Alamos, NM 87545 USA.
[Florando, J. N.; Kumar, M.] Lawrence Livermore Natl Lab, Livermore, CA 94550 USA.
RP Jones, DR (reprint author), Los Alamos Natl Lab, MST 8, Los Alamos, NM 87545 USA.
EM djones@lanl.gov
FU National Nuclear Security Administration of the U.S. Department of
Energy [DE-AC52-06NA25396]; Joint DoD/DoE Munitions Technology
Development Program; U.S. Department of Energy by Lawrence Livermore
National Laboratory [DE-AC52-07NA27344]
FX Los Alamos National Laboratory is operated by Los Alamos National
Security, LLC, for the National Nuclear Security Administration of the
U.S. Department of Energy under Contract No. DE-AC52-06NA25396. This
work was partially sponsored by the Joint DoD/DoE Munitions Technology
Development Program. Part of this work was performed under the auspices
of the U.S. Department of Energy by Lawrence Livermore National
Laboratory under Contract No. DE-AC52-07NA27344.
NR 31
TC 0
Z9 0
U1 14
U2 14
PU AMER INST PHYSICS
PI MELVILLE
PA 1305 WALT WHITMAN RD, STE 300, MELVILLE, NY 11747-4501 USA
SN 0021-8979
EI 1089-7550
J9 J APPL PHYS
JI J. Appl. Phys.
PD OCT 7
PY 2016
VL 120
IS 13
AR 135902
DI 10.1063/1.4963279
PG 8
WC Physics, Applied
SC Physics
GA DZ8XE
UT WOS:000386155100048
ER
PT J
AU Myers, SM
Wampler, WR
Modine, NA
AF Myers, Samuel M.
Wampler, William R.
Modine, Normand A.
TI Recombination by band-to-defect tunneling near semiconductor
heterojunctions: A theoretical model
SO JOURNAL OF APPLIED PHYSICS
LA English
DT Article
ID BIPOLAR-TRANSISTORS; COMPOUND SEMICONDUCTORS; SILICON; FIELD; GAAS
AB Carrier transport and recombination are modeled for a heterojunction diode containing irradiation defects. Detailed attention is given to the role of band-to-trap tunneling and how it is affected by band offsets at the junction. Tunneled states are characterized by numerical solution of the one-band effective-mass envelope equation. The interaction with traps is treated assuming capture by the multi-phonon-emission mechanism. It is shown that tunneling can increase carrier recombination at defects by orders of magnitude in the presence of large band offsets. This explains why Npn InGaP/GaAs/GaAs heterojunction bipolar transistors with displacement damage from energeticparticle irradiation are observed to have high carrier recombination in the emitter-base depletion region. Published by AIP Publishing.
C1 [Myers, Samuel M.; Wampler, William R.; Modine, Normand A.] Sandia Natl Labs, POB 5800, Albuquerque, NM 87185 USA.
RP Myers, SM (reprint author), Sandia Natl Labs, POB 5800, Albuquerque, NM 87185 USA.
FU U.S. Department of Energy's National Nuclear Security Administration
[DE-AC04-94AL85000]
FX A. Schenk and D. V. Lang provided valuable insights on carrier capture
by multi-phonon emission. A. F. Wright illuminated emerging theoretical
developments concerning irradiation defects in large-gap III-V alloys,
and also contributed to the development of our computational procedures.
Experimental Gummel plots from Sandia Laboratories were provided by Erin
Akinnikawe. This work was performed, in part, at the Center for
Integrated Nanotechnologies, an Office of Science User Facility operated
for the U.S. Department of Energy (DOE) Office of Science. Sandia
National Laboratories is a multi-program laboratory managed and operated
by Sandia Corporation, a wholly owned subsidiary of Lockheed Martin
Corporation, for the U.S. Department of Energy's National Nuclear
Security Administration under Contract No. DE-AC04-94AL85000.
NR 36
TC 0
Z9 0
U1 4
U2 4
PU AMER INST PHYSICS
PI MELVILLE
PA 1305 WALT WHITMAN RD, STE 300, MELVILLE, NY 11747-4501 USA
SN 0021-8979
EI 1089-7550
J9 J APPL PHYS
JI J. Appl. Phys.
PD OCT 7
PY 2016
VL 120
IS 13
AR 134502
DI 10.1063/1.4963873
PG 14
WC Physics, Applied
SC Physics
GA DZ8XE
UT WOS:000386155100021
ER
PT J
AU Swarnkar, A
Marshall, AR
Sanehira, EM
Chernomordik, BD
Moore, DT
Christians, JA
Chakrabarti, T
Luther, JM
AF Swarnkar, Abhishek
Marshall, Ashley R.
Sanehira, Erin M.
Chernomordik, Boris D.
Moore, David T.
Christians, Jeffrey A.
Chakrabarti, Tamoghna
Luther, Joseph M.
TI Quantum dot-induced phase stabilization of alpha-CsPbI3 perovskite for
high-efficiency photovoltaics
SO SCIENCE
LA English
DT Article
ID CESIUM-LEAD-HALIDE; OPTICAL-PROPERTIES; ROOM-TEMPERATURE; SOLAR-CELLS;
NANOCRYSTALS; EMISSION; NANOPARTICLES; LUMINESCENT; TRANSITION;
STABILITY
AB We show nanoscale phase stabilization of CsPbI3 quantum dots (QDs) to low temperatures that can be used as the active component of efficient optoelectronic devices. CsPbI3 is an all-inorganic analog to the hybrid organic cation halide perovskites, but the cubic phase of bulk CsPbI3 (alpha-CsPbI3)-the variant with desirable band gap-is only stable at high temperatures. We describe the formation of alpha-CsPbI3 QD films that are phase-stable for months in ambient air. The films exhibit long-range electronic transport and were used to fabricate colloidal perovskite QD photovoltaic cells with an open-circuit voltage of 1.23 volts and efficiency of 10.77%. These devices also function as light-emitting diodes with low turn-on voltage and tunable emission.
C1 [Swarnkar, Abhishek; Marshall, Ashley R.; Sanehira, Erin M.; Chernomordik, Boris D.; Moore, David T.; Christians, Jeffrey A.; Luther, Joseph M.] NREL, Chem & Mat Sci, Golden, CO 80401 USA.
[Swarnkar, Abhishek] IISER, Dept Chem, Pune 411008, Maharashtra, India.
[Marshall, Ashley R.] Univ Colorado, Dept Chem & Biochem, Boulder, CO 80309 USA.
[Sanehira, Erin M.] Univ Washington, Dept Elect Engn, Seattle, WA 98195 USA.
[Chakrabarti, Tamoghna] Colorado Sch Mines, Met & Mat Engn, Golden, CO 80401 USA.
RP Luther, JM (reprint author), NREL, Chem & Mat Sci, Golden, CO 80401 USA.
EM joey.luther@nrel.gov
FU U.S. Department of Energy, Office of Science, Office of Basic Energy
Sciences; U.S. Department of Energy, Office of Energy Efficiency and
Renewable Energy, Solar Energy Technologies Office
[DE-AC36-08GO28308DOE]; Department of Science and Technology, government
of India; Indo-U.S. Science and Technology Forum (IUSSTF); NASA Space
Technology Research Fellowship; NREL Director's Fellowship
FX We thank J. van de Lagemaat, W. Tumas, H. Choi, M. Beard, and J. Berry
for helpful discussions and B. To for SEM imaging. We acknowledge
support from the Center for Advanced Solar Photophysics, an Energy
Frontier Research Center funded by the U.S. Department of Energy, Office
of Science, Office of Basic Energy Sciences for quantum dot coupling and
solar cell structures. Device durability and structural phase
characterization was performed within the hybrid perovskite solar cell
program of the National Center for Photovoltaics funded by the U.S.
Department of Energy, Office of Energy Efficiency and Renewable Energy,
Solar Energy Technologies Office under contract DE-AC36-08GO28308DOE.
The original conception and QD synthesis was performed under the
Laboratory Directed Research and Development program at NREL. A.S.
acknowledges the Bhaskara Advanced Solar Energy fellowship funded by the
Department of Science and Technology, government of India, and Indo-U.S.
Science and Technology Forum (IUSSTF). E.M.S. acknowledges a NASA Space
Technology Research Fellowship. D.T.M. acknowledges the NREL Director's
Fellowship. All data in the paper and supplementary materials are
available. An application has been made for a provisional patent (U.S.
patent application no. 62/343,251).
NR 36
TC 30
Z9 30
U1 165
U2 165
PU AMER ASSOC ADVANCEMENT SCIENCE
PI WASHINGTON
PA 1200 NEW YORK AVE, NW, WASHINGTON, DC 20005 USA
SN 0036-8075
EI 1095-9203
J9 SCIENCE
JI Science
PD OCT 7
PY 2016
VL 354
IS 6308
SI SI
BP 92
EP 95
DI 10.1126/science.aag2700
PG 6
WC Multidisciplinary Sciences
SC Science & Technology - Other Topics
GA EC0GT
UT WOS:000387777900036
PM 27846497
ER
PT J
AU Desai, SB
Madhvapathy, SR
Sachid, AB
Llinas, JP
Wang, QX
Ahn, GH
Pitner, G
Kim, MJ
Bokor, J
Hu, CM
Wong, HSP
Javey, A
AF Desai, Sujay B.
Madhvapathy, Surabhi R.
Sachid, Angada B.
Llinas, Juan Pablo
Wang, Qingxiao
Ahn, Geun Ho
Pitner, Gregory
Kim, Moon J.
Bokor, Jeffrey
Hu, Chenming
Wong, H. -S. Philip
Javey, Ali
TI MoS2 transistors with 1-nanometer gate lengths
SO SCIENCE
LA English
DT Article
ID FIELD-EFFECT TRANSISTORS; CHANNEL-LENGTH; MOSFETS; EXTRACTION; JUNCTIONS
AB Scaling of silicon (Si) transistors is predicted to fail below 5-nanometer (nm) gate lengths because of severe short channel effects. As an alternative to Si, certain layered semiconductors are attractive for their atomically uniform thickness down to a monolayer, lower dielectric constants, larger band gaps, and heavier carrier effective mass. Here, we demonstrate molybdenum disulfide (MoS2) transistors with a 1-nm physical gate length using a single-walled carbon nanotube as the gate electrode. These ultrashort devices exhibit excellent switching characteristics with near ideal subthreshold swing of similar to 65 millivolts per decade and an On/Off current ratio of similar to 10(6). Simulations show an effective channel length of similar to 3.9 nm in the Off state and similar to 1 nm in the On state.
C1 [Desai, Sujay B.; Madhvapathy, Surabhi R.; Sachid, Angada B.; Llinas, Juan Pablo; Ahn, Geun Ho; Bokor, Jeffrey; Hu, Chenming; Javey, Ali] Univ Calif Berkeley, Elect Engn & Comp Sci, Berkeley, CA 94720 USA.
[Desai, Sujay B.; Madhvapathy, Surabhi R.; Sachid, Angada B.; Llinas, Juan Pablo; Ahn, Geun Ho; Bokor, Jeffrey; Javey, Ali] Lawrence Berkeley Natl Lab, Mat Sci Div, Berkeley, CA 94720 USA.
[Desai, Sujay B.; Javey, Ali] Univ Calif Berkeley, Berkeley Sensor & Actuator Ctr, Berkeley, CA 94720 USA.
[Wang, Qingxiao; Kim, Moon J.] Univ Texas Dallas, Dept Mat Sci & Engn, Richardson, TX 75080 USA.
[Pitner, Gregory; Wong, H. -S. Philip] Stanford Univ, Elect Engn, Stanford, CA 94305 USA.
RP Javey, A (reprint author), Univ Calif Berkeley, Elect Engn & Comp Sci, Berkeley, CA 94720 USA.; Javey, A (reprint author), Lawrence Berkeley Natl Lab, Mat Sci Div, Berkeley, CA 94720 USA.; Javey, A (reprint author), Univ Calif Berkeley, Berkeley Sensor & Actuator Ctr, Berkeley, CA 94720 USA.
EM ajavey@eecs.berkeley.edu
RI Kim, Moon/A-2297-2010
FU Electronics Materials program - Office of Science, Office of Basic
Energy Sciences, Materials Sciences and Engineering Division of the U.S.
Department of Energy [DE-AC02-05CH11231]; Applied Materials, Inc.;
Entegris, Inc., under the I-RiCE program; Office of Naval Research BRC
program; Berkeley Fellowship for Graduate Studies; NSF Graduate
Fellowship Program; NRI SWAN Center; Chinese Academy of Sciences
President's International Fellowship Initiative [2015VTA031]; SONIC
Research Center; STARnet phase of the Focus Center Research Program
(FCRP) a Semiconductor Research Corporation program - MARCO and DARPA;
Samsung
FX S.B.D. and A.J. were supported by the Electronics Materials program
funded by the Director, Office of Science, Office of Basic Energy
Sciences, Materials Sciences and Engineering Division of the U.S.
Department of Energy under contract DE-AC02-05CH11231. A.B.S. was funded
by Applied Materials, Inc., and Entegris, Inc., under the I-RiCE
program. J.P.L. and J.B. were supported in part by the Office of Naval
Research BRC program. J.P.L. acknowledges a Berkeley Fellowship for
Graduate Studies and the NSF Graduate Fellowship Program. Q.W. and
M.J.K. were supported by the NRI SWAN Center and Chinese Academy of
Sciences President's International Fellowship Initiative (2015VTA031).
G.P. and H.-S.P.W. were supported in part by the SONIC Research Center,
one of six centers supported by the STARnet phase of the Focus Center
Research Program (FCRP) a Semiconductor Research Corporation program
sponsored by MARCO and DARPA. A.J., H.-S.P.W., and J.B. acknowledge the
NSF Center for Energy Efficient Electronics Science (E3S). A.J.
acknowledges support from Samsung. The authors acknowledge the Molecular
Foundry, Lawrence Berkeley National Laboratory for access to the
scanning electron microscope. The authors acknowledge H. Fahad for
useful discussions about the analytical modeling. All data are reported
in the main text and supplementary materials.
NR 29
TC 10
Z9 10
U1 64
U2 64
PU AMER ASSOC ADVANCEMENT SCIENCE
PI WASHINGTON
PA 1200 NEW YORK AVE, NW, WASHINGTON, DC 20005 USA
SN 0036-8075
EI 1095-9203
J9 SCIENCE
JI Science
PD OCT 7
PY 2016
VL 354
IS 6308
SI SI
BP 99
EP 102
DI 10.1126/science.aah4698
PG 6
WC Multidisciplinary Sciences
SC Science & Technology - Other Topics
GA EC0GT
UT WOS:000387777900038
PM 27846499
ER
PT J
AU Dydio, P
Key, HM
Nazarenko, A
Rha, JYE
Seyedkazemi, V
Clark, DS
Hartwig, JF
AF Dydio, P.
Key, H. M.
Nazarenko, A.
Rha, J. Y. -E.
Seyedkazemi, V.
Clark, D. S.
Hartwig, J. F.
TI An artificial metalloenzyme with the kinetics of native enzymes
SO SCIENCE
LA English
DT Article
ID P450; CYTOCHROME-P450; HYDROXYLATION; CATALYSIS; IRON
AB Natural enzymes contain highly evolved active sites that lead to fast rates and high selectivities. Although artificial metalloenzymes have been developed that catalyze abiological transformations with high stereoselectivity, the activities of these artificial enzymes are much lower than those of natural enzymes. Here, we report a reconstituted artificial metalloenzyme containing an iridium porphyrin that exhibits kinetic parameters similar to those of natural enzymes. In particular, variants of the P450 enzyme CYP119 containing iridium in place of iron catalyze insertions of carbenes into C-H bonds with up to 98% enantiomeric excess, 35,000 turnovers, and 2550 hours-1 turnover frequency. This activity leads to intramolecular carbene insertions into unactivated C-H bonds and intermolecular carbene insertions into C-H bonds. These results lift the restrictions on merging chemical catalysis and biocatalysis to create highly active, productive, and selective metalloenzymes for abiological reactions.
C1 [Dydio, P.; Key, H. M.; Nazarenko, A.; Rha, J. Y. -E.; Seyedkazemi, V.; Hartwig, J. F.] Univ Calif Berkeley, Dept Chem, Berkeley, CA 94720 USA.
[Dydio, P.; Key, H. M.; Hartwig, J. F.] Lawrence Berkeley Natl Lab, Div Chem Sci, 1 Cyclotron Rd, Berkeley, CA 94720 USA.
[Clark, D. S.] Univ Calif Berkeley, Dept Chem & Biomol Engn, Berkeley, CA 94720 USA.
[Clark, D. S.] Lawrence Berkeley Natl Lab, Mol Biophys & Integrated Bioimaging Div, 1 Cyclotron Rd, Berkeley, CA 94720 USA.
RP Hartwig, JF (reprint author), Univ Calif Berkeley, Dept Chem, Berkeley, CA 94720 USA.; Hartwig, JF (reprint author), Lawrence Berkeley Natl Lab, Div Chem Sci, 1 Cyclotron Rd, Berkeley, CA 94720 USA.
EM jhartwig@berkeley.edu
FU Office of Science, of the U.S. Department of Energy [DE-AC02-05CH11231];
NSF; Netherlands Organization for Scientific Research [680-50-1306]; NIH
[1S10OD020062-01]
FX This work was supported by the Director, Office of Science, of the U.S.
Department of Energy under contract DE-AC02-05CH11231; by the NSF
(graduate research fellowship to H.M.K.), and the Netherlands
Organization for Scientific Research (the Rubicon postdoctoral
fellowship 680-50-1306 to P.D.). We thank the QB3 MacroLab facility
(competent cells), the University of California, Berkeley DNA Sequencing
Facility (plasmid sequencing), and T. Iavarone and the QB3 Mass
Spectrometry Facility [nano-electrospray ionization (NS-ESI) mass
spectrometry data collection, supported by NIH grant 1S10OD020062-01]
for native nanoESI-MS data and analysis. All data are provided in the
supplementary materials. J.F.H., H.M.K., P.F.D., and D.S.C. are
inventors on U.S. patent application numbers 62/241,487 and 62/384,011,
submitted by the Lawrence Berkeley National Laboratory, that covers
preparation and application of artificial metalloenzymes containing
noble metal-porphyrins.
NR 20
TC 5
Z9 6
U1 55
U2 55
PU AMER ASSOC ADVANCEMENT SCIENCE
PI WASHINGTON
PA 1200 NEW YORK AVE, NW, WASHINGTON, DC 20005 USA
SN 0036-8075
EI 1095-9203
J9 SCIENCE
JI Science
PD OCT 7
PY 2016
VL 354
IS 6308
SI SI
BP 102
EP 106
DI 10.1126/science.aah4427
PG 7
WC Multidisciplinary Sciences
SC Science & Technology - Other Topics
GA EC0GT
UT WOS:000387777900039
PM 27846500
ER
PT J
AU Nikolaienko, RM
Hammel, M
Dubreuil, V
Zalmai, R
Hall, DR
Mehzabeen, N
Karuppan, SJ
Harroch, S
Stella, SL
Bouyain, S
AF Nikolaienko, Roman M.
Hammel, Michal
Dubreuil, Veronique
Zalmai, Rana
Hall, David R.
Mehzabeen, Nurjahan
Karuppan, Sebastian J.
Harroch, Sheila
Stella, Salvatore L.
Bouyain, Samuel
TI Structural Basis for Interactions Between Contactin Family Members and
Protein-tyrosine Phosphatase Receptor Type G in Neural Tissues
SO JOURNAL OF BIOLOGICAL CHEMISTRY
LA English
DT Article
DE cell adhesion; cell surface; crystal structure; protein phosphatase;
retina; contactin; immunoglobulin|L-like domain
ID NUCLEOTIDE-GATED CHANNELS; RECOGNITION MOLECULES; EXTRACELLULAR REGION;
CRYSTAL-STRUCTURE; NERVOUS-SYSTEM; AXON GUIDANCE; RPTP-GAMMA; CELLS;
COMPLEX; CIS
AB Protein-tyrosine phosphatase receptor type G (RPTP/PTPRG) interacts in vitro with contactin-3-6 (CNTN3-6), a group of glycophosphatidylinositol-anchored cell adhesion molecules involved in the wiring of the nervous system. In addition to PTPRG, CNTNs associate with multiple transmembrane proteins and signal inside the cell via cis-binding partners to alleviate the absence of an intracellular region. Here, we use comprehensive biochemical and structural analyses to demonstrate that PTPRGCNTN3-6 complexes share similar binding affinities and a conserved arrangement. Furthermore, as a first step to identifying PTPRGCNTN complexes in vivo, we found that PTPRG and CNTN3 associate in the outer segments of mouse rod photoreceptor cells. In particular, PTPRG and CNTN3 form cis-complexes at the surface of photoreceptors yet interact in trans when expressed on the surfaces of apposing cells. Further structural analyses suggest that all CNTN ectodomains adopt a bent conformation and might lie parallel to the cell surface to accommodate these cis and trans binding modes. Taken together, these studies identify a PTPRGCNTN complex in vivo and provide novel insights into PTPRG- and CNTN-mediated signaling.
C1 [Nikolaienko, Roman M.; Zalmai, Rana; Hall, David R.; Mehzabeen, Nurjahan; Karuppan, Sebastian J.; Bouyain, Samuel] Univ Missouri, Sch Biol Sci, Div Mol Biol & Biochem, 5100 Rockhill Rd, Kansas City, MO 64110 USA.
[Hammel, Michal] Lawrence Berkeley Natl Lab, Div Life Sci, Berkeley, CA 94720 USA.
[Dubreuil, Veronique] Inst Pasteur Paris, Dept Neurosci, 25-28 Rue Dr Roux, F-75624 Paris, France.
[Dubreuil, Veronique; Harroch, Sheila] Univ Paris Diderot, CNRS, Sorbonne Paris Cite, Epigenet & Cell Fate,UMR 7216, Paris, France.
[Stella, Salvatore L.] Univ Missouri, Dept Basic Med Sci, Sch Med, Kansas City, MO 64108 USA.
[Harroch, Sheila] NYU, Sch Med, Dept Psychiat, 550 First Ave, New York, NY 10016 USA.
[Stella, Salvatore L.] Penn State Univ, Coll Med, Dept Neural & Behav Sci, 500 Univ Dr, Hershey, PA 17033 USA.
RP Bouyain, S (reprint author), Univ Missouri, Sch Biol Sci, Div Mol Biol & Biochem, 5100 Rockhill Rd, Kansas City, MO 64110 USA.
EM bouyains@umkc.edu
FU United States Department of Energy, Office of Science, Office of Basic
Energy Sciences [W-31-109-Eng-38]; United States Department of Energy
Program Integrated Diffraction Analysis Technologies (IDAT); National
Institutes of Health [MINOS GM105404]; NIGMS, National Institutes of
Health [P41-GM103311]
FX We thank Prof. Brian Geisbrecht for helpful comments on the manuscript
and assistance with circular dichroism. Use of the Advanced Photon
Source was supported by the United States Department of Energy, Office
of Science, Office of Basic Energy Sciences, under Contract
W-31-109-Eng-38. Data were collected at Southeast Regional Collaborative
Access Team beamlines at the Advanced Photon Source, Argonne National
Laboratory. Supporting institutions may be found at
www.ser-cat.org/members.html. X-ray scattering technologies at the
Lawrence Berkeley National Laboratory SIBYLS beamline of the Advanced
Light Source are supported in part by the United States Department of
Energy Program Integrated Diffraction Analysis Technologies (IDAT) and
National Institutes of Health Grant MINOS GM105404. Chimera was
developed by the Resource for Biocomputing, Visualization, and
Informatics at the University of California, San Francisco (supported by
NIGMS, National Institutes of Health, Grant P41-GM103311).
NR 61
TC 0
Z9 0
U1 0
U2 0
PU AMER SOC BIOCHEMISTRY MOLECULAR BIOLOGY INC
PI BETHESDA
PA 9650 ROCKVILLE PIKE, BETHESDA, MD 20814-3996 USA
SN 0021-9258
EI 1083-351X
J9 J BIOL CHEM
JI J. Biol. Chem.
PD OCT 7
PY 2016
VL 291
IS 41
BP 21335
EP 21349
DI 10.1074/jbc.M116.742163
PG 15
WC Biochemistry & Molecular Biology
SC Biochemistry & Molecular Biology
GA DZ6UX
UT WOS:000385999200001
PM 27539848
ER
PT J
AU Kawashima, N
Nishimiya, Y
Takahata, S
Nakayama, K
AF Kawashima, Nagako
Nishimiya, Yoshiyuki
Takahata, Shouta
Nakayama, Ken-ichi
TI Induction of Glycosphingolipid GM3 Expression by Valproic Acid
Suppresses Cancer Cell Growth
SO JOURNAL OF BIOLOGICAL CHEMISTRY
LA English
DT Article
DE cell proliferation; epidermal growth factor receptor (EGFR);
ganglioside; glycolipid; histone deacetylase inhibitor (HDAC inhibitor)
(HDI); GM3; glycosphingolipid; valproic acid
ID GANGLIOSIDE-MEDIATED MODULATION; TYROSINE KINASE-ACTIVITY; FACTOR
RECEPTOR; HISTONE DEACETYLASE; INSULIN-RECEPTOR; PHOSPHORYLATION;
SYNTHASE; GENE; DIFFERENTIATION; GLYCOLIPIDS
AB Glycosphingolipid GM3, a known suppressor of epidermal growth factor receptor (EGFR) phosphorylation, inhibits cell proliferation. Valproic acid, conversely, is known as an up-regulator of GM3 synthase gene (ST3GAL5). To test the possibility that valproic acid could inhibit EGFR phosphorylation by increasing the level of GM3 in cells, we treated A431 epidermoid carcinoma cells with valproic acid and found that valproic acid treatment caused an about 6-fold increase in the GM3 level but only a marginal increase in the GM2 level in these cells and that the observed increase in GM3 level was valproic acid dose-dependent. Consistent with this observation, valproic acid treatment induced GM3 synthase gene expression by about 8-fold. Furthermore, phosphorylation of EGFR was reduced, and cell proliferation was inhibited following valproic acid treatment. Consistent with these results, transient expression of GM3 synthase gene in A431 cells also increased cellular level of GM3, reduced phosphorylation of EGFR, and inhibited cell proliferation. Treatment with l-phenyl-2-decanoylamino-3-morpholino-l-propanol, an inhibitor of glucosylceramide synthesis, decreased the cellular level of GM3 and reduced the inhibitory effects of valproic acid on EGFR phosphorylation and cell proliferation. These results suggested that induction of GM3 synthesis was enough to inhibit proliferation of cancer cells by suppressing EGFR activity. Valproic acid treatment similarly increased the GM3 level and reduced phosphorylation of EGFR in U87MG glioma cells and inhibited their proliferation. These results suggested that up-regulators of GM3 synthase gene, such as valproic acid, are potential suppressors of cancer cell proliferation.
C1 [Kawashima, Nagako; Nishimiya, Yoshiyuki; Takahata, Shouta; Nakayama, Ken-ichi] Natl Inst Adv Ind Sci & Technol, Bioprod Res Inst, Sapporo, Hokkaido 0628517, Japan.
[Kawashima, Nagako] Pacific Northwest Res Inst, Div Biomembrane Res Inst, Seattle, WA 98122 USA.
[Nakayama, Ken-ichi] Natl Inst Adv Ind Sci & Technol, Res Inst Sustainable Chem, Hiroshima 7390046, Japan.
RP Nakayama, K (reprint author), Natl Inst Adv Ind Sci & Technol, Res Inst Sustainable Chem, Hiroshima 7390046, Japan.
EM k-nakayama@aist.go.jp
NR 26
TC 0
Z9 0
U1 0
U2 0
PU AMER SOC BIOCHEMISTRY MOLECULAR BIOLOGY INC
PI BETHESDA
PA 9650 ROCKVILLE PIKE, BETHESDA, MD 20814-3996 USA
SN 0021-9258
EI 1083-351X
J9 J BIOL CHEM
JI J. Biol. Chem.
PD OCT 7
PY 2016
VL 291
IS 41
BP 21424
EP 21433
DI 10.1074/jbc.M116.751503
PG 10
WC Biochemistry & Molecular Biology
SC Biochemistry & Molecular Biology
GA DZ6UX
UT WOS:000385999200011
PM 27539856
ER
PT J
AU Lehtola, S
Parkhill, J
Head-Gordon, M
AF Lehtola, Susi
Parkhill, John
Head-Gordon, Martin
TI Cost-effective description of strong correlation: Efficient
implementations of the perfect quadruples and perfect hextuples models
SO JOURNAL OF CHEMICAL PHYSICS
LA English
DT Article
ID MATRIX RENORMALIZATION-GROUP; COUPLED-CLUSTER METHOD; HIGHER-ORDER
TENSOR; QUANTUM-CHEMISTRY; WAVE-FUNCTIONS; AB-INITIO;
CONFIGURATION-INTERACTION; ELECTRON CORRELATION; MOLECULAR-ORBITALS; SCF
CALCULATIONS
AB Novel implementations based on dense tensor storage are presented for the singlet-reference perfect quadruples (PQ) [J. A. Parkhill et al., J. Chem. Phys. 130, 084101 (2009)] and perfect hextuples (PH) [J. A. Parkhill and M. Head-Gordon, J. Chem. Phys. 133, 024103 (2010)] models. The methods are obtained as block decompositions of conventional coupled-cluster theory that are exact for four electrons in four orbitals (PQ) and six electrons in six orbitals (PH), but that can also be applied to much larger systems. PQ and PH have storage requirements that scale as the square, and as the cube of the number of active electrons, respectively, and exhibit quartic scaling of the computational effort for large systems. Applications of the new implementations are presented for full-valence calculations on linear polyenes (CnHn+2), which highlight the excellent computational scaling of the present implementations that can routinely handle active spaces of hundreds of electrons. The accuracy of the models is studied in the pi space of the polyenes, in hydrogen chains (H-50), and in the pi space of polyacene molecules. In all cases, the results compare favorably to density matrix renormalization group values. With the novel implementation of PQ, active spaces of 140 electrons in 140 orbitals can be solved in a matter of minutes on a single core workstation, and the relatively low polynomial scaling means that very large systems are also accessible using parallel computing. Published by AIP Publishing.
C1 [Lehtola, Susi; Head-Gordon, Martin] Lawrence Berkeley Natl Lab, Chem Sci Div, Berkeley, CA 94720 USA.
[Parkhill, John] Univ Notre Dame, Dept Chem, 251 Nieuwland Sci Hall, Notre Dame, IN 46556 USA.
[Head-Gordon, Martin] Univ Calif Berkeley, Dept Chem, Berkeley, CA 94720 USA.
RP Lehtola, S (reprint author), Lawrence Berkeley Natl Lab, Chem Sci Div, Berkeley, CA 94720 USA.
EM susi.lehtola@alumni.helsinki.fi; john.parkhill@gmail.com;
mhg@cchem.berkeley.edu
RI Lehtola, Susi/H-1828-2013
OI Lehtola, Susi/0000-0001-6296-8103
FU Office of Basic Energy Sciences, Chemical Sciences, Geosciences, and
Biosciences Division of the U.S. Department of Energy
[DE-AC02-05CH11231]; University of Notre Dame's College of Science;
University of Notre Dame's Department of Chemistry and Biochemistry
FX S.L. thanks Evgeny Epifanovsky, David Small, and Joonho Lee for
discussions, and Johannes Hachmann for supplying the DMRG natural
occupation numbers for the polyacenes. This work was supported by the
Director, Office of Basic Energy Sciences, Chemical Sciences,
Geosciences, and Biosciences Division of the U.S. Department of Energy,
under Contract No. DE-AC02-05CH11231. J.P. thanks the University of
Notre Dame's College of Science and Department of Chemistry and
Biochemistry for generous start-up funding.
NR 71
TC 1
Z9 1
U1 12
U2 12
PU AMER INST PHYSICS
PI MELVILLE
PA 1305 WALT WHITMAN RD, STE 300, MELVILLE, NY 11747-4501 USA
SN 0021-9606
EI 1089-7690
J9 J CHEM PHYS
JI J. Chem. Phys.
PD OCT 7
PY 2016
VL 145
IS 13
AR 134110
DI 10.1063/1.4964317
PG 11
WC Chemistry, Physical; Physics, Atomic, Molecular & Chemical
SC Chemistry; Physics
GA DZ8XP
UT WOS:000386156200013
PM 27782439
ER
PT J
AU Radak, BK
Roux, B
AF Radak, Brian K.
Roux, Benoit
TI Efficiency in nonequilibrium molecular dynamics Monte Carlo simulations
SO JOURNAL OF CHEMICAL PHYSICS
LA English
DT Article
ID FREE-ENERGY DIFFERENCES; ENTROPY; THEOREM; MODEL
AB Hybrid algorithms combining nonequilibrium molecular dynamics and Monte Carlo (neMD/MC) offer a powerful avenue for improving the sampling efficiency of computer simulations of complex systems. These neMD/MC algorithms are also increasingly finding use in applications where conventional approaches are impractical, such as constant-pH simulations with explicit solvent. However, selecting an optimal nonequilibrium protocol for maximum efficiency often represents a non-trivial challenge. This work evaluates the efficiency of a broad class of neMD/MC algorithms and protocols within the theoretical framework of linear response theory. The approximations are validated against constant pH-MD simulations and shown to provide accurate predictions of neMD/MC performance. An assessment of a large set of protocols confirms (both theoretically and empirically) that a linear work protocol gives the best neMD/MC performance. Finally, a well-defined criterion for optimizing the time parameters of the protocol is proposed and demonstrated with an adaptive algorithm that improves the performance on-the-fly with minimal cost. Published by AIP Publishing.
C1 [Radak, Brian K.] Argonne Natl Lab, Leadership Comp Facil, 9700 S Cass Ave, Argonne, IL 60439 USA.
[Roux, Benoit] Univ Chicago, Dept Biochem & Mol Biol, 920 E 58Th St, Chicago, IL 60637 USA.
[Roux, Benoit] Argonne Natl Lab, Ctr Nanoscale Mat, 9700 S Cass Ave, Argonne, IL 60439 USA.
RP Radak, BK (reprint author), Argonne Natl Lab, Leadership Comp Facil, 9700 S Cass Ave, Argonne, IL 60439 USA.
EM brian.radak@anl.gov; roux@uchicago.edu
OI Radak, Brian/0000-0001-8628-5972
FU Theta Early Science Program; National Institutes of Health
[U54-GM087519]; [DE-AC02-06CH11357]
FX This research was supported under the Theta Early Science Program and
used resources of the Argonne Leadership Computing Facility, which is a
DOE Oce of Science User Facility supported under Contract
DE-AC02-06CH11357. This work was also supported in part by the National
Institutes of Health Grant No. U54-GM087519 (to B.R.) and by resources
provided by the University of Chicago Research Computing Center. The
authors are grateful to Yunjie Chen and John Chodera (Memorial
Sloan-Kettering Cancer Center) for many helpful discussions.
NR 32
TC 0
Z9 0
U1 5
U2 5
PU AMER INST PHYSICS
PI MELVILLE
PA 1305 WALT WHITMAN RD, STE 300, MELVILLE, NY 11747-4501 USA
SN 0021-9606
EI 1089-7690
J9 J CHEM PHYS
JI J. Chem. Phys.
PD OCT 7
PY 2016
VL 145
IS 13
AR 134109
DI 10.1063/1.4964288
PG 6
WC Chemistry, Physical; Physics, Atomic, Molecular & Chemical
SC Chemistry; Physics
GA DZ8XP
UT WOS:000386156200012
PM 27782441
ER
PT J
AU Qian, F
Lan, PC
Olson, T
Zhu, C
Duoss, EB
Spadaccini, CM
Han, TYJ
AF Qian, Fang
Lan, Pui Ching
Olson, Tammy
Zhu, Cheng
Duoss, Eric B.
Spadaccini, Christopher M.
Han, T. Yong-Jin
TI Multiphase separation of copper nanowires
SO CHEMICAL COMMUNICATIONS
LA English
DT Article
ID CONDUCTING FILMS; SILVER NANOWIRES; HIGH-PERFORMANCE; TRANSPARENT
CONDUCTORS; RAPID SYNTHESIS; CU NANOWIRES; PURIFICATION; ELECTRODES;
NETWORKS
AB This communication reports a new method to purify copper nano wires with nearly 100% yield from undesired copper nanoparticle side-products formed during batch processes of copper nanowire synthesis. This simple separation method can yield large quantities of long, uniform, high-purity copper nanowires to meet the requirements of nanoelectronics applications as well as provide an avenue for purifying copper nanowires in the industrial scale synthesis of copper nanowires, a key step for commercialization and application of nanowires.
C1 [Qian, Fang; Lan, Pui Ching; Olson, Tammy; Han, T. Yong-Jin] Lawrence Livermore Natl Lab, Phys & Life Sci Directorate, Livermore, CA 94550 USA.
[Zhu, Cheng; Duoss, Eric B.; Spadaccini, Christopher M.] Lawrence Livermore Natl Lab, Engn Directorate, Livermore, CA 94550 USA.
RP Han, TYJ (reprint author), Lawrence Livermore Natl Lab, Phys & Life Sci Directorate, Livermore, CA 94550 USA.
EM han5@llnl.gov
FU Lawrence Livermore National Laboratory under the auspices of the U.S.
Department of Energy [DE-AC52-07NA27344]; LDRD award [13-ER-022 and
14-SI-004]
FX We thank Dr Zurong Dai for TEM characterization. This work was supported
by Lawrence Livermore National Laboratory under the auspices of the U.S.
Department of Energy under Contract DE-AC52-07NA27344, through LDRD
award 13-ER-022 and 14-SI-004.
NR 18
TC 0
Z9 0
U1 59
U2 59
PU ROYAL SOC CHEMISTRY
PI CAMBRIDGE
PA THOMAS GRAHAM HOUSE, SCIENCE PARK, MILTON RD, CAMBRIDGE CB4 0WF, CAMBS,
ENGLAND
SN 1359-7345
EI 1364-548X
J9 CHEM COMMUN
JI Chem. Commun.
PD OCT 7
PY 2016
VL 52
IS 78
BP 11627
EP 11630
DI 10.1039/c6cc06228h
PG 4
WC Chemistry, Multidisciplinary
SC Chemistry
GA DY9SP
UT WOS:000385475700002
PM 27711287
ER
PT J
AU Li, CK
Tzeferacos, P
Lamb, D
Gregori, G
Norreys, PA
Rosenberg, MJ
Follett, RK
Froula, DH
Koenig, M
Seguin, FH
Frenje, JA
Rinderknecht, HG
Sio, H
Zylstra, AB
Petrasso, RD
Amendt, PA
Park, HS
Remington, BA
Ryutov, DD
Wilks, SC
Betti, R
Frank, A
Hu, SX
Sangster, TC
Hartigan, P
Drake, RP
Kuranz, CC
Lebedev, SV
Woolsey, NC
AF Li, C. K.
Tzeferacos, P.
Lamb, D.
Gregori, G.
Norreys, P. A.
Rosenberg, M. J.
Follett, R. K.
Froula, D. H.
Koenig, M.
Seguin, F. H.
Frenje, J. A.
Rinderknecht, H. G.
Sio, H.
Zylstra, A. B.
Petrasso, R. D.
Amendt, P. A.
Park, H. S.
Remington, B. A.
Ryutov, D. D.
Wilks, S. C.
Betti, R.
Frank, A.
Hu, S. X.
Sangster, T. C.
Hartigan, P.
Drake, R. P.
Kuranz, C. C.
Lebedev, S. V.
Woolsey, N. C.
TI Scaled laboratory experiments explain the kink behaviour of the Crab
Nebula jet
SO NATURE COMMUNICATIONS
LA English
DT Article
ID CONFINEMENT-FUSION PLASMAS; MAGNETOHYDRODYNAMIC SIMULATIONS;
MAGNETIC-FIELDS; VELA PULSAR; Z-PINCH; ASTROPHYSICS; INSTABILITY
AB The remarkable discovery by the Chandra X-ray observatory that the Crab nebula's jet periodically changes direction provides a challenge to our understanding of astrophysical jet dynamics. It has been suggested that this phenomenon may be the consequence of magnetic fields and magnetohydrodynamic instabilities, but experimental demonstration in a controlled laboratory environment has remained elusive. Here we report experiments that use high-power lasers to create a plasma jet that can be directly compared with the Crab jet through well-defined physical scaling laws. The jet generates its own embedded toroidal magnetic fields; as it moves, plasma instabilities result in multiple deflections of the propagation direction, mimicking the kink behaviour of the Crab jet. The experiment is modelled with three-dimensional numerical simulations that show exactly how the instability develops and results in changes of direction of the jet.
C1 [Li, C. K.; Rosenberg, M. J.; Seguin, F. H.; Frenje, J. A.; Rinderknecht, H. G.; Sio, H.; Zylstra, A. B.; Petrasso, R. D.] MIT, Plasma Sci & Fus Ctr, 77 Massachusetts Ave, Cambridge, MA 02139 USA.
[Tzeferacos, P.; Lamb, D.] Univ Chicago, Dept Astron & Astrophys, 5640 South Ellis Ave, Chicago, IL 60637 USA.
[Gregori, G.; Norreys, P. A.] Univ Oxford, Dept Phys, Parks Rd, Oxford OX1 3PU, England.
[Follett, R. K.; Froula, D. H.; Betti, R.; Frank, A.; Hu, S. X.; Sangster, T. C.] Univ Rochester, Laser Energet Lab, 250 E River Rd, Rochester, NY 14627 USA.
[Follett, R. K.; Froula, D. H.; Betti, R.; Frank, A.] Univ Rochester, Dept Phys & Astron, Rochester, NY 14627 USA.
[Koenig, M.] CEA, Ecole Polytech, LULI CNRS, F-91128 Palaiseau, France.
[Koenig, M.] Univ Paris Saclay, F-91128 Palaiseau, France.
[Koenig, M.] Univ Paris 06, F-91128 Palaiseau, France.
[Koenig, M.] Sorbonne Univ, F-91128 Palaiseau, France.
[Koenig, M.] Osaka Univ, Inst Laser Engn, Suita, Osaka 5650871, Japan.
[Amendt, P. A.; Park, H. S.; Remington, B. A.; Ryutov, D. D.; Wilks, S. C.] Lawrence Livermore Natl Lab, Livermore, CA 94551 USA.
[Hartigan, P.] Rice Univ, Dept Phys & Astron, 6100 S Main, Houston, TX 77521 USA.
[Drake, R. P.; Kuranz, C. C.] Univ Michigan, Dept Atmospher Ocean & Space Sci, 2455 Hayward St, Ann Arbor, MI 48103 USA.
[Lebedev, S. V.] Imperial Coll London, Blackett Lab, London SW7 2BW, England.
[Woolsey, N. C.] Univ York, Dept Phys, York YO10 5D, N Yorkshire, England.
RP Li, CK (reprint author), MIT, Plasma Sci & Fus Ctr, 77 Massachusetts Ave, Cambridge, MA 02139 USA.
EM ckli@mit.edu
RI Hu, Suxing/A-1265-2007
OI Hu, Suxing/0000-0003-2465-3818
FU US DOE [DE-FG03-09NA29553, DE-SC0007168]; LLE [414090-G]; NLUF
[DE-NA0000877]; FSC [415023-G]; LLNL [B580243]; US DOE NNSA ASC [57789];
Computation Institute; Biological Sciences Division of the University of
Chicago; Argonne National Laboratory [1S10OD018495-01]; European
Research Council under the European Community [256973]; DOE Office of
Science User Facility [DE-AC02-06CH11357]
FX We thank the OMEGA operations and target fabrication crews for their
assistance in carrying out these experiments and R. Frankel, and E. Doeg
for their help in processing of CR-39 data used in this work. The
experiments were supported in part by US DOE (Grant No.
DE-FG03-09NA29553, No. DE-SC0007168), LLE (No. 414090-G), NLUF (No.
DE-NA0000877), FSC (No. 415023-G) and LLNL (No. B580243). Numerical
simulations were supported in part by the US DOE NNSA ASC under Field
Work Proposal No. 57789 to the Argonne National Laboratory, and by NIH
through resources provided by the Computation Institute and the
Biological Sciences Division of the University of Chicago and Argonne
National Laboratory (Grant 1S10OD018495-01). Partial support from the
European Research Council under the European Community's Seventh
Framework Programme (FP7/2007-2013)/ERC grant agreements no. 256973 is
acknowledged. The software used in this work was developed in part by
the DOE NNSA ASC- and DOE Office of Science ASCR-supported Flash Center
for Computational Science at the University of Chicago. This research
used resources from the Director's Discretionary Program of the Argonne
Leadership Computing Facility, supported by DOE Office of Science User
Facility (DE-AC02-06CH11357).
NR 44
TC 0
Z9 0
U1 16
U2 16
PU NATURE PUBLISHING GROUP
PI LONDON
PA MACMILLAN BUILDING, 4 CRINAN ST, LONDON N1 9XW, ENGLAND
SN 2041-1723
J9 NAT COMMUN
JI Nat. Commun.
PD OCT 7
PY 2016
VL 7
AR 13081
DI 10.1038/ncomms13081
PG 8
WC Multidisciplinary Sciences
SC Science & Technology - Other Topics
GA DZ1GV
UT WOS:000385587800001
PM 27713403
ER
PT J
AU Qin, N
Zhang, SQ
Jiang, JJ
Gilbert Corder, S
Qian, ZG
Zhou, ZT
Lee, W
Liu, KY
Wang, XH
Li, XX
Shi, ZF
Mao, Y
Bechtel, HA
Martin, MC
Xia, XX
Marelli, B
Kaplan, DL
Omenetto, FG
Liu, MK
Tao, TH
AF Qin, Nan
Zhang, Shaoqing
Jiang, Jianjuan
Gilbert Corder, Stephanie
Qian, Zhigang
Zhou, Zhitao
Lee, Woonsoo
Liu, Keyin
Wang, Xiaohan
Li, Xinxin
Shi, Zhifeng
Mao, Ying
Bechtel, Hans A.
Martin, Michael C.
Xia, Xiaoxia
Marelli, Benedetto
Kaplan, David L.
Omenetto, Fiorenzo G.
Liu, Mengkun
Tao, Tiger H.
TI Nanoscale probing of electron-regulated structural transitions in silk
proteins by near-field IR imaging and nano-spectroscopy
SO NATURE COMMUNICATIONS
LA English
DT Article
ID INFRARED NANOSPECTROSCOPY; FIBROIN; LITHOGRAPHY; ABSORPTION; MICROSCOPY;
RESOLUTION; RESIST; FILMS
AB Silk protein fibres produced by silkworms and spiders are renowned for their unparalleled mechanical strength and extensibility arising from their high-beta-sheet crystal contents as natural materials. Investigation of beta-sheet-oriented conformational transitions in silk proteins at the nanoscale remains a challenge using conventional imaging techniques given their limitations in chemical sensitivity or limited spatial resolution. Here, we report on electron-regulated nanoscale polymorphic transitions in silk proteins revealed by near-field infrared imaging and nano-spectroscopy at resolutions approaching the molecular level. The ability to locally probe nanoscale protein structural transitions combined with nanometre-precision electron-beam lithography offers us the capability to finely control the structure of silk proteins in two and three dimensions. Our work paves the way for unlocking essential nanoscopic protein structures and critical conditions for electron-induced conformational transitions, offering new rules to design protein-based nanoarchitectures.
C1 [Qin, Nan; Jiang, Jianjuan; Zhou, Zhitao; Liu, Keyin; Li, Xinxin; Tao, Tiger H.] Chinese Acad Sci, Shanghai Inst Microsyst & Informat Technol, State Key Lab Transducer Technol, Shanghai 200050, Peoples R China.
[Zhang, Shaoqing; Lee, Woonsoo; Wang, Xiaohan; Tao, Tiger H.] Univ Texas Austin, Dept Mech Engn, Austin, TX 78712 USA.
[Gilbert Corder, Stephanie; Liu, Mengkun] SUNY Stony Brook, Dept Phys & Astron, Stony Brook, NY 11794 USA.
[Qian, Zhigang; Xia, Xiaoxia] Shanghai Jiao Tong Univ, Sch Life Sci & Biotechnol, State Key Lab Microbial Metab, Shanghai 200240, Peoples R China.
[Li, Xinxin; Tao, Tiger H.] ShanghaiTech Univ, Sch Phys Sci & Technol, Shanghai 200031, Peoples R China.
[Shi, Zhifeng; Mao, Ying] Fudan Univ, Dept Neurosurg, Huashan Hosp, Wulumuqi Zhong Rd 12, Shanghai 200040, Peoples R China.
[Bechtel, Hans A.; Martin, Michael C.] Lawrence Berkeley Natl Lab, Adv Light Source Div, Nano FTIR, Berkeley, CA 94720 USA.
[Marelli, Benedetto] MIT, Dept Civil & Environm Engn, Cambridge, MA 02139 USA.
[Kaplan, David L.; Omenetto, Fiorenzo G.] Tufts Univ, Dept Biomed Engn, Medford, MA 02155 USA.
[Kaplan, David L.] Tufts Univ, Dept Chem Engn, Medford, MA 02155 USA.
[Omenetto, Fiorenzo G.] Tufts Univ, Dept Phys, Medford, MA 02155 USA.
RP Tao, TH (reprint author), Chinese Acad Sci, Shanghai Inst Microsyst & Informat Technol, State Key Lab Transducer Technol, Shanghai 200050, Peoples R China.; Tao, TH (reprint author), Univ Texas Austin, Dept Mech Engn, Austin, TX 78712 USA.; Liu, MK (reprint author), SUNY Stony Brook, Dept Phys & Astron, Stony Brook, NY 11794 USA.; Tao, TH (reprint author), ShanghaiTech Univ, Sch Phys Sci & Technol, Shanghai 200031, Peoples R China.; Omenetto, FG (reprint author), Tufts Univ, Dept Biomed Engn, Medford, MA 02155 USA.; Omenetto, FG (reprint author), Tufts Univ, Dept Phys, Medford, MA 02155 USA.
EM fiorenzo.omenetto@tufts.edu; mengkun.liu@stonybrook.edu;
tiger.tao@austin.utexas.edu
RI Gilbert Corder, Stephanie/F-3658-2015; Qian, Zhi-Gang/G-4519-2012; Xia,
Xiaoxia/C-6614-2013; Qin, Nan/D-5374-2017;
OI Gilbert Corder, Stephanie/0000-0002-5041-8670; Qian,
Zhi-Gang/0000-0002-0133-0605; Xia, Xiaoxia/0000-0001-8375-1616; Wang,
Xiaohan/0000-0003-2608-0718; Marelli, Benedetto/0000-0001-5311-6961
FU National Natural Science Foundation of China [61574156, 61527818]; MOST
of China [2016YFA0200800]; National Basic Research Program of China (973
Program) [2015CB755500]; International Science AMP; Technology
Cooperation Program of China [2014DFA31470]; Science and Technology
Commission of Shanghai Municipality [14520720400]; NSF under the CMMI
Division [1563422, 1562915]
FX The work has been partially supported by the National Natural Science
Foundation of China (Grant No. 61574156, No. 61527818), MOST of China
(Grant No. 2016YFA0200800), the National Basic Research Program of China
(973 Program, 2015CB755500), the International Science & Technology
Cooperation Program of China (2014DFA31470) and the Science and
Technology Commission of Shanghai Municipality for the support under the
International Collaboration Project (Grant No. 14520720400). We thank
the NSF for support under the CMMI Division (Grant No. 1563422 &
1562915). We acknowledge K. Kjoller & A. Roy (Anasys Instruments, USA)
and Professor M.B. Raschke (JILA, University of Colorado, USA) for their
support on IR nano-spectroscopic measurements. T.H.T. and M.L. thank S.
Mastel & A. Huber (Neaspec GmbH, Germany) and G. Andreev (Evanescent
Solutions, USA) for helpful discussion. T.H.T. thanks Professor Keji Lai
(UT Austin) for helpful discussion and Professor Yaguo Wang (UT Austin)
for her precious support on instrumental set up.
NR 40
TC 1
Z9 1
U1 40
U2 40
PU NATURE PUBLISHING GROUP
PI LONDON
PA MACMILLAN BUILDING, 4 CRINAN ST, LONDON N1 9XW, ENGLAND
SN 2041-1723
J9 NAT COMMUN
JI Nat. Commun.
PD OCT 7
PY 2016
VL 7
AR 13079
DI 10.1038/ncomms13079
PG 8
WC Multidisciplinary Sciences
SC Science & Technology - Other Topics
GA DZ1GR
UT WOS:000385587400001
PM 27713412
ER
PT J
AU Adamson, P
An, FP
Anghel, I
Aurisano, A
Balantekin, AB
Band, HR
Barr, G
Bishai, M
Blake, A
Blyth, S
Bock, GJ
Bogert, D
Cao, D
Cao, GF
Cao, J
Cao, SV
Carroll, TJ
Castromonte, CM
Cen, WR
Chan, YL
Chang, JF
Chang, LC
Chang, Y
Chen, HS
Chen, QY
Chen, R
Chen, SM
Chen, Y
Chen, YX
Cheng, J
Cheng, JH
Cheng, YP
Cheng, ZK
Cherwinka, JJ
Childress, S
Chu, MC
Chukanov, A
Coelho, JAB
Corwin, L
Cronin-Hennessy, D
Cummings, JP
de Arcos, J
De Rijck, S
Deng, ZY
Devan, AV
Devenish, NE
Ding, XF
Ding, YY
Diwan, MV
Dolgareva, M
Dove, J
Dwyer, DA
Edwards, WR
Escobar, CO
Evans, JJ
Falk, E
Feldman, GJ
Flanagan, W
Frohne, MV
Gabrielyan, M
Gallagher, HR
Germani, S
Gill, R
Gomes, RA
Gonchar, M
Gong, GH
Gong, H
Goodman, MC
Gouffon, P
Graf, N
Gran, R
Grassi, M
Grzelak, K
Gu, WQ
Guan, MY
Guo, L
Guo, RP
Guo, XH
Guo, Z
Habig, A
Hackenburg, RW
Hahn, SR
Han, R
Hans, S
Hartnell, J
Hatcher, R
He, M
Heeger, KM
Heng, YK
Higuera, A
Holin, A
Hor, YK
Hsiung, YB
Hu, BZ
Hu, T
Hu, W
Huang, EC
Huang, HX
Huang, J
Huang, XT
Huber, P
Huo, W
Hussain, G
Hylen, J
Irwin, GM
Isvan, Z
Jaffe, DE
Jaffke, P
James, C
Jen, KL
Jensen, D
Jetter, S
Ji, XL
Ji, XP
Jiao, JB
Johnson, RA
de Jong, JK
Joshi, J
Kafka, T
Kang, L
Kasahara, SMS
Kettell, SH
Kohn, S
Koizumi, G
Kordosky, M
Kramer, M
Kreymer, A
Kwan, KK
Kwok, MW
Kwok, T
Lang, K
Langford, TJ
Lau, K
Lebanowski, L
Lee, J
Lee, JHC
Lei, RT
Leitner, R
Leung, JKC
Li, C
Li, DJ
Li, F
Li, GS
Li, QJ
Li, S
Li, SC
Li, WD
Li, XN
Li, YF
Li, ZB
Liang, H
Lin, CJ
Lin, GL
Lin, S
Lin, SK
Lin, YC
Ling, JJ
Link, JM
Litchfield, PJ
Littenberg, L
Littlejohn, BR
Liu, DW
Liu, JC
Liu, JL
Loh, CW
Lu, C
Lu, HQ
Lu, JS
Lucas, P
Luk, KB
Lv, Z
Ma, QM
Ma, XB
Ma, XY
Ma, YQ
Malyshkin, Y
Mann, WA
Marshak, ML
Caicedo, DAM
Mayer, N
McDonald, KT
McGivern, C
McKeown, RD
Medeiros, MM
Mehdiyev, R
Meier, JR
Messier, MD
Miller, WH
Mishra, SR
Mitchell, I
Mooney, M
Moore, CD
Mualem, L
Musser, J
Nakajima, Y
Naples, D
Napolitano, J
Naumov, D
Naumova, E
Nelson, JK
Newman, HB
Ngai, HY
Nichol, RJ
Ning, Z
Nowak, JA
O'Connor, J
Ochoa-Ricoux, JP
Olshevskiy, A
Orchanian, M
Pahlka, RB
Paley, J
Pan, HR
Park, J
Patterson, RB
Patton, S
Pawloski, G
Pec, V
Peng, JC
Perch, A
Pfutzner, MM
Phan, DD
Phan-Budd, S
Pinsky, L
Plunkett, RK
Poonthottathil, N
Pun, CSJ
Qi, FZ
Qi, M
Qian, X
Qiu, X
Radovic, A
Raper, N
Rebel, B
Ren, J
Rosenfeld, C
Rosero, R
Roskovec, B
Ruan, XC
Rubin, HA
Sail, P
Sanchez, MC
Schneps, J
Schreckenberger, A
Schreiner, P
Sharma, R
Sher, SM
Sousa, A
Steiner, H
Sun, GX
Sun, JL
Tagg, N
Talaga, RL
Tang, W
Taychenachev, D
Thomas, J
Thomson, MA
Tian, X
Timmons, A
Todd, J
Tognini, SC
Toner, R
Torretta, D
Treskov, K
Tsang, KV
Tull, CE
Tzanakos, G
Urheim, J
Vahle, P
Viaux, N
Viren, B
Vorobel, V
Wang, CH
Wang, M
Wang, NY
Wang, RG
Wang, W
Wang, X
Wang, YF
Wang, Z
Wang, ZM
Webb, RC
Weber, A
Wei, HY
Wen, LJ
Whisnant, K
White, C
Whitehead, L
Whitehead, LH
Wise, T
Wojcicki, SG
Wong, HLH
Wong, SCF
Worcester, E
Wu, CH
Wu, Q
Wu, WJ
Xia, DM
Xia, JK
Xing, ZZ
Xu, JL
Xu, JY
Xu, Y
Xue, T
Yang, CG
Yang, H
Yang, L
Yang, MS
Yang, MT
Ye, M
Ye, Z
Yeh, M
Young, BL
Yu, ZY
Zeng, S
Zhan, L
Zhang, C
Zhang, HH
Zhang, JW
Zhang, QM
Zhang, XT
Zhang, YM
Zhang, YX
Zhang, ZJ
Zhang, ZP
Zhang, ZY
Zhao, J
Zhao, QW
Zhao, YB
Zhong, WL
Zhou, L
Zhou, N
Zhuang, HL
Zou, JH
AF Adamson, P.
An, F. P.
Anghel, I.
Aurisano, A.
Balantekin, A. B.
Band, H. R.
Barr, G.
Bishai, M.
Blake, A.
Blyth, S.
Bock, G. J.
Bogert, D.
Cao, D.
Cao, G. F.
Cao, J.
Cao, S. V.
Carroll, T. J.
Castromonte, C. M.
Cen, W. R.
Chan, Y. L.
Chang, J. F.
Chang, L. C.
Chang, Y.
Chen, H. S.
Chen, Q. Y.
Chen, R.
Chen, S. M.
Chen, Y.
Chen, Y. X.
Cheng, J.
Cheng, J. -H.
Cheng, Y. P.
Cheng, Z. K.
Cherwinka, J. J.
Childress, S.
Chu, M. C.
Chukanov, A.
Coelho, J. A. B.
Corwin, L.
Cronin-Hennessy, D.
Cummings, J. P.
de Arcos, J.
De Rijck, S.
Deng, Z. Y.
Devan, A. V.
Devenish, N. E.
Ding, X. F.
Ding, Y. Y.
Diwan, M. V.
Dolgareva, M.
Dove, J.
Dwyer, D. A.
Edwards, W. R.
Escobar, C. O.
Evans, J. J.
Falk, E.
Feldman, G. J.
Flanagan, W.
Frohne, M. V.
Gabrielyan, M.
Gallagher, H. R.
Germani, S.
Gill, R.
Gomes, R. A.
Gonchar, M.
Gong, G. H.
Gong, H.
Goodman, M. C.
Gouffon, P.
Graf, N.
Gran, R.
Grassi, M.
Grzelak, K.
Gu, W. Q.
Guan, M. Y.
Guo, L.
Guo, R. P.
Guo, X. H.
Guo, Z.
Habig, A.
Hackenburg, R. W.
Hahn, S. R.
Han, R.
Hans, S.
Hartnell, J.
Hatcher, R.
He, M.
Heeger, K. M.
Heng, Y. K.
Higuera, A.
Holin, A.
Hor, Y. K.
Hsiung, Y. B.
Hu, B. Z.
Hu, T.
Hu, W.
Huang, E. C.
Huang, H. X.
Huang, J.
Huang, X. T.
Huber, P.
Huo, W.
Hussain, G.
Hylen, J.
Irwin, G. M.
Isvan, Z.
Jaffe, D. E.
Jaffke, P.
James, C.
Jen, K. L.
Jensen, D.
Jetter, S.
Ji, X. L.
Ji, X. P.
Jiao, J. B.
Johnson, R. A.
de Jong, J. K.
Joshi, J.
Kafka, T.
Kang, L.
Kasahara, S. M. S.
Kettell, S. H.
Kohn, S.
Koizumi, G.
Kordosky, M.
Kramer, M.
Kreymer, A.
Kwan, K. K.
Kwok, M. W.
Kwok, T.
Lang, K.
Langford, T. J.
Lau, K.
Lebanowski, L.
Lee, J.
Lee, J. H. C.
Lei, R. T.
Leitner, R.
Leung, J. K. C.
Li, C.
Li, D. J.
Li, F.
Li, G. S.
Li, Q. J.
Li, S.
Li, S. C.
Li, W. D.
Li, X. N.
Li, Y. F.
Li, Z. B.
Liang, H.
Lin, C. J.
Lin, G. L.
Lin, S.
Lin, S. K.
Lin, Y. -C.
Ling, J. J.
Link, J. M.
Litchfield, P. J.
Littenberg, L.
Littlejohn, B. R.
Liu, D. W.
Liu, J. C.
Liu, J. L.
Loh, C. W.
Lu, C.
Lu, H. Q.
Lu, J. S.
Lucas, P.
Luk, K. B.
Lv, Z.
Ma, Q. M.
Ma, X. B.
Ma, X. Y.
Ma, Y. Q.
Malyshkin, Y.
Mann, W. A.
Marshak, M. L.
Caicedo, D. A. Martinez
Mayer, N.
McDonald, K. T.
McGivern, C.
McKeown, R. D.
Medeiros, M. M.
Mehdiyev, R.
Meier, J. R.
Messier, M. D.
Miller, W. H.
Mishra, S. R.
Mitchell, I.
Mooney, M.
Moore, C. D.
Mualem, L.
Musser, J.
Nakajima, Y.
Naples, D.
Napolitano, J.
Naumov, D.
Naumova, E.
Nelson, J. K.
Newman, H. B.
Ngai, H. Y.
Nichol, R. J.
Ning, Z.
Nowak, J. A.
O'Connor, J.
Ochoa-Ricoux, J. P.
Olshevskiy, A.
Orchanian, M.
Pahlka, R. B.
Paley, J.
Pan, H. -R.
Park, J.
Patterson, R. B.
Patton, S.
Pawloski, G.
Pec, V.
Peng, J. C.
Perch, A.
Pfuetzner, M. M.
Phan, D. D.
Phan-Budd, S.
Pinsky, L.
Plunkett, R. K.
Poonthottathil, N.
Pun, C. S. J.
Qi, F. Z.
Qi, M.
Qian, X.
Qiu, X.
Radovic, A.
Raper, N.
Rebel, B.
Ren, J.
Rosenfeld, C.
Rosero, R.
Roskovec, B.
Ruan, X. C.
Rubin, H. A.
Sail, P.
Sanchez, M. C.
Schneps, J.
Schreckenberger, A.
Schreiner, P.
Sharma, R.
Sher, S. Moed
Sousa, A.
Steiner, H.
Sun, G. X.
Sun, J. L.
Tagg, N.
Talaga, R. L.
Tang, W.
Taychenachev, D.
Thomas, J.
Thomson, M. A.
Tian, X.
Timmons, A.
Todd, J.
Tognini, S. C.
Toner, R.
Torretta, D.
Treskov, K.
Tsang, K. V.
Tull, C. E.
Tzanakos, G.
Urheim, J.
Vahle, P.
Viaux, N.
Viren, B.
Vorobel, V.
Wang, C. H.
Wang, M.
Wang, N. Y.
Wang, R. G.
Wang, W.
Wang, X.
Wang, Y. F.
Wang, Z.
Wang, Z. M.
Webb, R. C.
Weber, A.
Wei, H. Y.
Wen, L. J.
Whisnant, K.
White, C.
Whitehead, L.
Whitehead, L. H.
Wise, T.
Wojcicki, S. G.
Wong, H. L. H.
Wong, S. C. F.
Worcester, E.
Wu, C. -H.
Wu, Q.
Wu, W. J.
Xia, D. M.
Xia, J. K.
Xing, Z. Z.
Xu, J. L.
Xu, J. Y.
Xu, Y.
Xue, T.
Yang, C. G.
Yang, H.
Yang, L.
Yang, M. S.
Yang, M. T.
Ye, M.
Ye, Z.
Yeh, M.
Young, B. L.
Yu, Z. Y.
Zeng, S.
Zhan, L.
Zhang, C.
Zhang, H. H.
Zhang, J. W.
Zhang, Q. M.
Zhang, X. T.
Zhang, Y. M.
Zhang, Y. X.
Zhang, Z. J.
Zhang, Z. P.
Zhang, Z. Y.
Zhao, J.
Zhao, Q. W.
Zhao, Y. B.
Zhong, W. L.
Zhou, L.
Zhou, N.
Zhuang, H. L.
Zou, J. H.
CA Daya Bay Collaboration
MINOS Collaboration
TI Limits on Active to Sterile Neutrino Oscillations from Disappearance
Searches in the MINOS, Daya Bay, and Bugey-3 Experiments
SO PHYSICAL REVIEW LETTERS
LA English
DT Article
ID REACTOR; SPECTRUM
AB Searches for a light sterile neutrino have been performed independently by the MINOS and the Daya Bay experiments using the muon (anti) neutrino and electron antineutrino disappearance channels, respectively. In this Letter, results from both experiments are combined with those from the Bugey-3 reactor neutrino experiment to constrain oscillations into light sterile neutrinos. The three experiments are sensitive to complementary regions of parameter space, enabling the combined analysis to probe regions allowed by the Liquid Scintillator Neutrino Detector (LSND) and MiniBooNE experiments in a minimally extended four-neutrino flavor framework. Stringent limits on sin(2) 2 theta(mu e) are set over 6 orders of magnitude in the sterile mass-squared splitting Delta m(41)(2). The sterile-neutrino mixing phase space allowed by the LSND and MiniBooNE experiments is excluded for Delta m(41)(2) < 0.8 eV(2) at 95% CLs.
C1 [Adamson, P.; Bock, G. J.; Bogert, D.; Childress, S.; Hahn, S. R.; Hatcher, R.; Hylen, J.; James, C.; Jensen, D.; Koizumi, G.; Kreymer, A.; Lucas, P.; Moore, C. D.; Pahlka, R. B.; Plunkett, R. K.; Poonthottathil, N.; Rebel, B.; Sharma, R.; Sher, S. Moed; Torretta, D.] Fermilab Natl Accelerator Lab, Batavia, IL 60510 USA.
[An, F. P.] East China Univ Sci & Technol, Inst Modern Phys, Shanghai, Peoples R China.
[Anghel, I.; Sanchez, M. C.; Whisnant, K.; Young, B. L.] Iowa State Univ, Dept Phys & Astron, Ames, IA 50011 USA.
[Anghel, I.; Goodman, M. C.; Paley, J.; Phan-Budd, S.; Sanchez, M. C.; Schreiner, P.; Talaga, R. L.] Argonne Natl Lab, Argonne, IL 60439 USA.
[Aurisano, A.; Johnson, R. A.; Sousa, A.; Todd, J.] Univ Cincinnati, Dept Phys, Cincinnati, OH 45221 USA.
[Balantekin, A. B.; Cherwinka, J. J.; Wise, T.] Univ Wisconsin, Dept Phys, Madison, WI 53706 USA.
[Band, H. R.; Heeger, K. M.; Langford, T. J.] Yale Univ, Dept Phys, New Haven, CT 06520 USA.
[Barr, G.; de Jong, J. K.; Weber, A.] Univ Oxford, Subdept Particle Phys, Oxford OX1 3RH, England.
[Bishai, M.; Diwan, M. V.; Gill, R.; Hackenburg, R. W.; Hans, S.; Isvan, Z.; Jaffe, D. E.; Joshi, J.; Kettell, S. H.; Ling, J. J.; Littenberg, L.; Mooney, M.; Qian, X.; Rosero, R.; Tang, W.; Viren, B.; Worcester, E.; Yang, M. S.; Yeh, M.; Zhang, C.] Brookhaven Natl Lab, Upton, NY 11973 USA.
[Blake, A.; Thomson, M. A.] Univ Cambridge, Cavendish Lab, Cambridge CB3 0HE, England.
[Blake, A.] Univ Lancaster, Lancaster LA1 4YB, England.
[Blyth, S.; Hsiung, Y. B.; Hu, B. Z.; Lin, Y. -C.; Pan, H. -R.] Natl Taiwan Univ, Dept Phys, Taipei, Taiwan.
[Blyth, S.; Chang, Y.; Wang, C. H.] Natl United Univ, Miaoli, Taiwan.
[Cao, D.; Loh, C. W.; Qi, M.; Yang, H.] Nanjing Univ, Nanjing, Jiangsu, Peoples R China.
[Cao, G. F.; Cao, J.; Cen, W. R.; Chang, J. F.; Chen, H. S.; Cheng, Y. P.; Deng, Z. Y.; Ding, X. F.; Ding, Y. Y.; Grassi, M.; Guan, M. Y.; Guo, R. P.; He, M.; Heng, Y. K.; Hu, T.; Hu, W.; Jetter, S.; Ji, X. L.; Li, F.; Li, Q. J.; Li, W. D.; Li, X. N.; Li, Y. F.; Liu, J. C.; Lu, H. Q.; Lu, J. S.; Ma, Q. M.; Ma, X. Y.; Ma, Y. Q.; Ning, Z.; Qi, F. Z.; Sun, G. X.; Wang, R. G.; Wang, Y. F.; Wang, Z.; Wang, Z. M.; Wen, L. J.; Wu, W. J.; Xia, J. K.; Xing, Z. Z.; Xu, J. L.; Yang, C. G.; Yang, L.; Ye, M.; Yu, Z. Y.; Zeng, S.; Zhan, L.; Zhang, J. W.; Zhang, X. T.; Zhang, Z. Y.; Zhao, J.; Zhao, Q. W.; Zhao, Y. B.; Zhong, W. L.; Zhou, L.; Zhuang, H. L.; Zou, J. H.] Inst High Energy Phys, Beijing, Peoples R China.
[Cao, S. V.; Carroll, T. J.; De Rijck, S.; Flanagan, W.; Huang, J.; Lang, K.; Mehdiyev, R.; Phan, D. D.; Sail, P.; Schreckenberger, A.] Univ Texas Austin, Dept Phys, Austin, TX 78712 USA.
[Castromonte, C. M.; Gomes, R. A.; Medeiros, M. M.; Tognini, S. C.] Univ Fed Goias, Inst Fis, BR-74690900 Goiania, Go, Brazil.
[Chan, Y. L.; Chu, M. C.; Kwan, K. K.; Kwok, M. W.; Xu, J. Y.] Chinese Univ Hong Kong, Hong Kong, Hong Kong, Peoples R China.
[Chang, L. C.; Cheng, J. -H.; Jen, K. L.; Lin, G. L.; Wu, C. -H.] Natl Chiao Tung Univ, Inst Phys, Hsinchu, Taiwan.
[Chen, Q. Y.; Cheng, J.; Huang, X. T.; Jiao, J. B.; Li, C.; Wang, M.; Wu, Q.] Shandong Univ, Jinan, Peoples R China.
[Chen, R.; Evans, J. J.; Timmons, A.] Univ Manchester, Sch Phys & Astron, Manchester M13 9PL, Lancs, England.
[Chen, S. M.; Gong, G. H.; Gong, H.; Guo, L.; Guo, Z.; Hussain, G.; Ji, X. P.; Lebanowski, L.; Wei, H. Y.; Xue, T.] Tsinghua Univ, Dept Engn Phys, Beijing, Peoples R China.
[Chen, Y.] Shenzhen Univ, Shenzhen, Peoples R China.
[Chen, Y. X.; Han, R.; Ma, X. B.] North China Elect Power Univ, Beijing, Peoples R China.
[Cheng, Z. K.; Li, Z. B.; Ling, J. J.; Wang, W.; Wong, S. C. F.; Xu, Y.; Yang, M. T.; Zhang, H. H.; Zhang, Y. M.] Sun Yat Sen Zhongshan Univ, Guangzhou, Guangdong, Peoples R China.
[Chukanov, A.; Dolgareva, M.; Gonchar, M.; Naumov, D.; Naumova, E.; Olshevskiy, A.; Taychenachev, D.; Treskov, K.] Joint Inst Nucl Res, Dubna, Moscow Region, Russia.
[Coelho, J. A. B.; Gallagher, H. R.; Kafka, T.; Mann, W. A.; Mayer, N.; Schneps, J.] Tufts Univ, Dept Phys, Medford, MA 02155 USA.
[Corwin, L.; Messier, M. D.; Musser, J.; Urheim, J.] Indiana Univ, Bloomington, IN 47405 USA.
[Cronin-Hennessy, D.; Gabrielyan, M.; Kasahara, S. M. S.; Litchfield, P. J.; Marshak, M. L.; Meier, J. R.; Miller, W. H.; Nowak, J. A.; Pawloski, G.] Univ Minnesota, Minneapolis, MN 55455 USA.
[Cummings, J. P.] Siena Coll, Loudonville, NY 12211 USA.
[de Arcos, J.; Littlejohn, B. R.; Caicedo, D. A. Martinez; Rubin, H. A.; White, C.] IIT, Dept Phys, Chicago, IL 60616 USA.
[Devan, A. V.; Kordosky, M.; McKeown, R. D.; Nelson, J. K.; Radovic, A.; Vahle, P.; Wang, W.] Coll William & Mary, Dept Phys, Williamsburg, VA 23187 USA.
[Devenish, N. E.; Falk, E.; Hartnell, J.; Kramer, M.] Univ Sussex, Dept Phys & Astron, Brighton BN1 9QH, E Sussex, England.
[Dove, J.; Huang, E. C.; Peng, J. C.] Univ Illinois, Dept Phys, Urbana, IL 61801 USA.
[Dwyer, D. A.; Edwards, W. R.; Kramer, M.; Lee, J.; Lin, C. J.; Luk, K. B.; Nakajima, Y.; Patton, S.; Tsang, K. V.; Tull, C. E.] Lawrence Berkeley Natl Lab0, Berkeley, CA 94720 USA.
[Escobar, C. O.] Univ Estadual Campinas, IFGW, CP 6165, BR-13083970 Campinas, SP, Brazil.
[Feldman, G. J.; Toner, R.] Harvard Univ, Dept Phys, Cambridge, MA 02138 USA.
[Frohne, M. V.] Coll Holy Cross, Notre Dame, IN 46556 USA.
[Germani, S.; Holin, A.; Nichol, R. J.; O'Connor, J.; Perch, A.; Pfuetzner, M. M.; Thomas, J.; Whitehead, L. H.] UCL, Dept Phys & Astron, London WC1E 6BT, England.
[Gouffon, P.] Univ Sao Paulo, Inst Fis, CP 66318, BR-05315970 Sao Paulo, SP, Brazil.
[Graf, N.; McGivern, C.; Naples, D.] Univ Pittsburgh, Dept Phys & Astron, Pittsburgh, PA 15260 USA.
[Gran, R.; Habig, A.] Univ Minnesota, Dept Phys, Duluth, MN 55812 USA.
[Grzelak, K.] Univ Warsaw, Dept Phys, PL-02093 Warsaw, Poland.
[Gu, W. Q.; Li, G. S.; Liu, J. L.] Shanghai Jiao Tong Univ, Dept Phys & Astron, Shanghai Lab Particle Phys & Cosmol, Shanghai, Peoples R China.
[Guo, X. H.; Wang, N. Y.] Beijing Normal Univ, Beijing, Peoples R China.
[Higuera, A.; Lau, K.; Lin, S. K.; Liu, D. W.; Mitchell, I.; Pinsky, L.; Whitehead, L.; Ye, Z.] Univ Houston, Dept Phys, Houston, TX 77204 USA.
[Hor, Y. K.; Huber, P.; Jaffke, P.; Li, S. C.; Link, J. M.; Park, J.] Virginia Tech, Ctr Neutrino Phys, Blacksburg, VA 24061 USA.
[Huang, H. X.; Ren, J.; Ruan, X. C.] China Inst Atom Energy, Beijing, Peoples R China.
[Huo, W.; Li, D. J.; Liang, H.; Zhang, Z. P.; Zhou, N.] Univ Sci & Technol China, Hefei, Peoples R China.
[Irwin, G. M.; Qiu, X.; Wojcicki, S. G.] Stanford Univ, Dept Phys, Stanford, CA 94305 USA.
[Ji, X. P.] Nankai Univ, Sch Phys, Tianjin, Peoples R China.
[Kang, L.; Lei, R. T.; Li, S.; Lin, S.; Zhang, Z. J.] Dongguan Univ Technol, Dongguan, Peoples R China.
[Kohn, S.; Luk, K. B.; Steiner, H.; Wong, H. L. H.] Univ Calif Berkeley, Dept Phys, Berkeley, CA 94720 USA.
[Kwok, T.; Lee, J. H. C.; Leung, J. K. C.; Li, S. C.; Ngai, H. Y.; Pun, C. S. J.] Univ Hong Kong, Dept Phys, Pokfulam, Hong Kong, Peoples R China.
[Leitner, R.; Pec, V.; Roskovec, B.; Steiner, H.; Vorobel, V.; Wong, H. L. H.] Charles Univ Prague, Fac Math & Phys, Prague, Czech Republic.
[Litchfield, P. J.; Weber, A.] Rutherford Appleton Lab, Sci & Technol Facil Council, Didcot OX11 0QX, Oxon, England.
[Lu, C.; McDonald, K. T.] Princeton Univ, Joseph Henry Labs, Princeton, NJ 08544 USA.
[Lv, Z.; Zhang, Q. M.] Xi An Jiao Tong Univ, Xian, Peoples R China.
[Malyshkin, Y.; Ochoa-Ricoux, J. P.; Viaux, N.] Pontificia Univ Catolica Chile, Inst Fis, Santiago, Chile.
[McKeown, R. D.; Mualem, L.; Newman, H. B.; Orchanian, M.; Patterson, R. B.] CALTECH, Lauritsen Lab, Pasadena, CA 91125 USA.
[Mishra, S. R.; Rosenfeld, C.; Tian, X.] Univ South Carolina, Dept Phys & Astron, Columbia, SC 29208 USA.
[Napolitano, J.] Temple Univ, Coll Sci & Technol, Dept Phys, Philadelphia, PA 19122 USA.
[Raper, N.] Rensselaer Polytech Inst, Dept Phys Appl Phys & Astron, Troy, NY 12180 USA.
[Sun, J. L.; Zhang, Y. X.] China Gen Nucl Power Grp, Shenzhen, Guangdong, Peoples R China.
[Tagg, N.] Otterbein Univ, Westerville, OH 43081 USA.
[Tzanakos, G.] Univ Athens, Dept Phys, GR-15771 Athens, Greece.
[Wang, X.] Natl Univ Def Technol, Coll Elect Sci & Engn, Changsha, Hunan, Peoples R China.
[Webb, R. C.] Texas A&M Univ, Dept Phys, College Stn, TX 77843 USA.
[Xia, D. M.] Chongqing Univ, Chongqing, Peoples R China.
RP Adamson, P (reprint author), Fermilab Natl Accelerator Lab, Batavia, IL 60510 USA.
RI Ling, Jiajie/I-9173-2014; Gomes, Ricardo/B-6899-2008; Leitner,
Rupert/C-2004-2017; Liu, Jianglai/P-2587-2015;
OI Nowak, Jaroslaw/0000-0001-8637-5433; Ling, Jiajie/0000-0003-2982-0670;
Gomes, Ricardo/0000-0003-0278-4876; Weber, Alfons/0000-0002-8222-6681;
Ochoa-Ricoux, Juan Pedro/0000-0001-7376-5555; Leitner,
Rupert/0000-0002-2994-2187; Liu, Jianglai/0000-0002-4563-3157; Hartnell,
Jeffrey/0000-0002-1744-7955; Qian, Xin/0000-0002-7903-7935; Zhang,
Chao/0000-0003-2298-6272; Castromonte Flores, Cesar
Manuel/0000-0002-9559-3704; Grassi, Marco/0000-0003-2422-6736
FU U.S. Department of Energy; United Kingdom Science and Technology
Facilities Council; U.S. National Science Foundation; State and
University of Minnesota; Brazil FAPESP (Fundacao de Amparo a Pesquisa do
Estado de Sao Paulo); Brazil CNPq (Conselho Nacional de Desenvolvimento
Cientifico e Tecnologico); Brazil CAPES (Coordenacao de Aperfeicoamento
de Pessoal de Nivel Superior); Ministry of Science and Technology of
China; Chinese Academy of Sciences; CAS Center for Excellence in
Particle Physics; National Natural Science Foundation of China;
Guangdong provincial government; Shenzhen municipal government; China
General Nuclear Power Group; Research Grants Council of the Hong Kong
Special Administrative Region of China; Ministry of Education in Taiwan;
Ministry of Education, Youth and Sports of the Czech Republic; Joint
Institute of Nuclear Research in Dubna, Russia; NSFC-RFBR joint research
program; National Commission for Scientific and Technological Research
of Chile
FX The MINOS experiment is supported by the U.S. Department of Energy, the
United Kingdom Science and Technology Facilities Council, the U.S.
National Science Foundation, the State and University of Minnesota, and
Brazil's FAPESP (Fundacao de Amparo a Pesquisa do Estado de Sao Paulo),
CNPq (Conselho Nacional de Desenvolvimento Cientifico e Tecnologico),
and CAPES (Coordenacao de Aperfeicoamento de Pessoal de Nivel Superior).
We are grateful to the Minnesota Department of Natural Resources and the
personnel of the Soudan Laboratory and Fermilab. We thank the Texas
Advanced Computing Center at The University of Texas at Austin for the
provision of computing resources. The Daya Bay experiment is supported
in part by the Ministry of Science and Technology of China, the U.S.
Department of Energy, the Chinese Academy of Sciences, the CAS Center
for Excellence in Particle Physics, the National Natural Science
Foundation of China, the Guangdong provincial government, the Shenzhen
municipal government, the China General Nuclear Power Group, the
Research Grants Council of the Hong Kong Special Administrative Region
of China, the Ministry of Education in Taiwan, the U.S. National Science
Foundation, the Ministry of Education, Youth and Sports of the Czech
Republic, the Joint Institute of Nuclear Research in Dubna, Russia, the
NSFC-RFBR joint research program, and the National Commission for
Scientific and Technological Research of Chile. We acknowledge Yellow
River Engineering Consulting Co., Ltd. and China Railway 15th Bureau
Group Co., Ltd. for building the underground laboratory. We are grateful
for the ongoing cooperation from the China Guangdong Nuclear Power Group
and China Light & Power Company.
NR 49
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PU AMER PHYSICAL SOC
PI COLLEGE PK
PA ONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA
SN 0031-9007
EI 1079-7114
J9 PHYS REV LETT
JI Phys. Rev. Lett.
PD OCT 7
PY 2016
VL 117
IS 15
AR 151801
DI 10.1103/PhysRevLett.117.151801
PG 9
WC Physics, Multidisciplinary
SC Physics
GA DY7XF
UT WOS:000385341900006
PM 27768356
ER
PT J
AU Adamson, P
Anghel, I
Aurisano, A
Barr, G
Bishai, M
Blake, A
Bock, GJ
Bogert, D
Cao, SV
Carroll, TJ
Castromonte, CM
Chen, R
Childress, S
Coelho, JAB
Corwin, L
Cronin-Hennessy, D
de Jong, JK
De Rijck, S
Devan, AV
Devenish, NE
Diwan, MV
Escobar, CO
Evans, JJ
Falk, E
Feldman, GJ
Flanagan, W
Frohne, MV
Gabrielyan, M
Gallagher, HR
Germani, S
Gomes, RA
Goodman, MC
Gouffon, P
Graf, N
Gran, R
Grzelak, K
Habig, A
Hahn, SR
Hartnell, J
Hatcher, R
Holin, A
Huang, J
Hylen, J
Irwin, GM
Isvan, Z
James, C
Jensen, D
Kafka, T
Kasahara, SMS
Koizumi, G
Kordosky, M
Kreymer, A
Lang, K
Ling, J
Litchfield, PJ
Lucas, P
Mann, WA
Marshak, ML
Mayer, N
McGivern, C
Medeiros, MM
Mehdiyev, R
Meier, JR
Messier, MD
Miller, WH
Mishra, SR
Sher, SM
Moore, CD
Mualem, L
Musser, J
Naples, D
Nelson, JK
Newman, HB
Nichol, RJ
Nowak, JA
O'Connor, J
Orchanian, M
Pahlka, RB
Paley, J
Patterson, RB
Pawloski, G
Perch, A
Pfutzner, MM
Phan, DD
Phan-Budd, S
Plunkett, RK
Poonthottathil, N
Qiu, X
Radovic, A
Rebel, B
Rosenfeld, C
Rubin, HA
Sail, P
Sanchez, MC
Schneps, J
Schreckenberger, A
Schreiner, P
Sharma, R
Sousa, A
Tagg, N
Talaga, RL
Thomas, J
Thomson, MA
Tian, X
Timmons, A
Todd, J
Tognini, SC
Toner, R
Torretta, D
Tzanakos, G
Urheim, J
Vahle, P
Viren, B
Weber, A
Webb, RC
White, C
Whitehead, L
Whitehead, LH
Wojcicki, SG
Zwaska, R
AF Adamson, P.
Anghel, I.
Aurisano, A.
Barr, G.
Bishai, M.
Blake, A.
Bock, G. J.
Bogert, D.
Cao, S. V.
Carroll, T. J.
Castromonte, C. M.
Chen, R.
Childress, S.
Coelho, J. A. B.
Corwin, L.
Cronin-Hennessy, D.
de Jong, J. K.
De Rijck, S.
Devan, A. V.
Devenish, N. E.
Diwan, M. V.
Escobar, C. O.
Evans, J. J.
Falk, E.
Feldman, G. J.
Flanagan, W.
Frohne, M. V.
Gabrielyan, M.
Gallagher, H. R.
Germani, S.
Gomes, R. A.
Goodman, M. C.
Gouffon, P.
Graf, N.
Gran, R.
Grzelak, K.
Habig, A.
Hahn, S. R.
Hartnell, J.
Hatcher, R.
Holin, A.
Huang, J.
Hylen, J.
Irwin, G. M.
Isvan, Z.
James, C.
Jensen, D.
Kafka, T.
Kasahara, S. M. S.
Koizumi, G.
Kordosky, M.
Kreymer, A.
Lang, K.
Ling, J.
Litchfield, P. J.
Lucas, P.
Mann, W. A.
Marshak, M. L.
Mayer, N.
McGivern, C.
Medeiros, M. M.
Mehdiyev, R.
Meier, J. R.
Messier, M. D.
Miller, W. H.
Mishra, S. R.
Sher, S. Moed
Moore, C. D.
Mualem, L.
Musser, J.
Naples, D.
Nelson, J. K.
Newman, H. B.
Nichol, R. J.
Nowak, J. A.
O'Connor, J.
Orchanian, M.
Pahlka, R. B.
Paley, J.
Patterson, R. B.
Pawloski, G.
Perch, A.
Pfuetzner, M. M.
Phan, D. D.
Phan-Budd, S.
Plunkett, R. K.
Poonthottathil, N.
Qiu, X.
Radovic, A.
Rebel, B.
Rosenfeld, C.
Rubin, H. A.
Sail, P.
Sanchez, M. C.
Schneps, J.
Schreckenberger, A.
Schreiner, P.
Sharma, R.
Sousa, A.
Tagg, N.
Talaga, R. L.
Thomas, J.
Thomson, M. A.
Tian, X.
Timmons, A.
Todd, J.
Tognini, S. C.
Toner, R.
Torretta, D.
Tzanakos, G.
Urheim, J.
Vahle, P.
Viren, B.
Weber, A.
Webb, R. C.
White, C.
Whitehead, L.
Whitehead, L. H.
Wojcicki, S. G.
Zwaska, R.
CA MINOS Collaboration
TI Search for Sterile Neutrinos Mixing with Muon Neutrinos in MINOS
SO PHYSICAL REVIEW LETTERS
LA English
DT Article
ID OSCILLATIONS
AB We report results of a search for oscillations involving a light sterile neutrino over distances of 1.04 and 735 km in a nu(mu)-dominated beam with a peak energy of 3 GeV. The data, from an exposure of 10.56 x 10(20) protons on target, are analyzed using a phenomenological model with one sterile neutrino. We constrain the mixing parameters theta(24) and Delta m(41)(2) and set limits on parameters of the four-dimensional Pontecorvo-Maki-Nakagawa-Sakata matrix, vertical bar U-mu 4 vertical bar(2) and vertical bar U-tau 4 vertical bar(2), under the assumption that mixing between nu(e) and nu(s) is negligible (vertical bar U-e4 vertical bar(2) = 0). No evidence for nu(mu) -> nu(s) transitions is found and we set a world-leading limit on theta(24) for values of Delta m(41)(2) less than or similar to 1 eV(2).
C1 [Anghel, I.; Goodman, M. C.; Paley, J.; Phan-Budd, S.; Sanchez, M. C.; Schreiner, P.; Talaga, R. L.] Argonne Natl Lab, Argonne, IL 60439 USA.
[Tzanakos, G.] Univ Athens, Dept Phys, GR-15771 Athens, Greece.
[Bishai, M.; Diwan, M. V.; Isvan, Z.; Ling, J.; Viren, B.] Brookhaven Natl Lab, Upton, NY 11973 USA.
[Mualem, L.; Newman, H. B.; Orchanian, M.; Patterson, R. B.] CALTECH, Lauritsen Lab, Pasadena, CA 91125 USA.
[Blake, A.; Thomson, M. A.] Univ Cambridge, Cavendish Lab, Cambridge CB3 0HE, England.
[Escobar, C. O.] Univ Estadual Campinas, IFGW, CP 6165, BR-13083970 Campinas, SP, Brazil.
[Aurisano, A.; Sousa, A.; Todd, J.] Univ Cincinnati, Dept Phys, Cincinnati, OH 45221 USA.
[Adamson, P.; Bock, G. J.; Bogert, D.; Childress, S.; Hahn, S. R.; Hatcher, R.; Hylen, J.; James, C.; Jensen, D.; Koizumi, G.; Kreymer, A.; Lucas, P.; Sher, S. Moed; Moore, C. D.; Pahlka, R. B.; Plunkett, R. K.; Poonthottathil, N.; Rebel, B.; Sharma, R.; Torretta, D.; Zwaska, R.] Fermilab Natl Accelerator Lab, Batavia, IL 60510 USA.
[Castromonte, C. M.; Gomes, R. A.; Medeiros, M. M.; Tognini, S. C.] Univ Fed Goias, Inst Fis, BR-74690900 Goiania, Go, Brazil.
[Feldman, G. J.; Toner, R.] Harvard Univ, Dept Phys, Cambridge, MA 02138 USA.
[Frohne, M. V.] Coll Holy Cross, Notre Dame, IN 46556 USA.
[Whitehead, L.] Univ Houston, Dept Phys, Houston, TX 77204 USA.
[Rubin, H. A.; White, C.] IIT, Dept Phys, Chicago, IL 60616 USA.
[Corwin, L.; Messier, M. D.; Musser, J.; Urheim, J.] Indiana Univ, Bloomington, IN 47405 USA.
[Anghel, I.; Sanchez, M. C.] Iowa State Univ, Dept Phys & Astron, Ames, IA 50011 USA.
[Blake, A.] Univ Lancaster, Lancaster LA1 4YB, England.
[Germani, S.; Holin, A.; Nichol, R. J.; O'Connor, J.; Perch, A.; Pfuetzner, M. M.; Thomas, J.; Whitehead, L. H.] UCL, Dept Phys & Astron, London WC1E 6BT, England.
[Chen, R.; Evans, J. J.; Timmons, A.] Univ Manchester, Sch Phys & Astron, Manchester M13 9PL, Lancs, England.
[Cronin-Hennessy, D.; Gabrielyan, M.; Kasahara, S. M. S.; Litchfield, P. J.; Marshak, M. L.; Meier, J. R.; Miller, W. H.; Nowak, J. A.; Pawloski, G.] Univ Minnesota, Minneapolis, MN 55455 USA.
[Gran, R.; Habig, A.] Univ Minnesota, Dept Phys, Duluth, MN 55812 USA.
[Tagg, N.] Otterbein Univ, Westerville, OH 43081 USA.
[Barr, G.; de Jong, J. K.; Weber, A.] Univ Oxford, Subdept Particle Phys, Oxford OX1 3RH, England.
[Graf, N.; McGivern, C.; Naples, D.] Univ Pittsburgh, Dept Phys & Astron, Pittsburgh, PA 15260 USA.
[Litchfield, P. J.; Weber, A.] Rutherford Appleton Lab, Sci & Technol Facil Council, Didcot OX11 0QX, Oxon, England.
[Gouffon, P.] Univ Sao Paulo, Inst Fis, CP 66318, BR-05315970 Sao Paulo, SP, Brazil.
[Mishra, S. R.; Rosenfeld, C.; Tian, X.] Univ South Carolina, Dept Phys & Astron, Columbia, SC 29208 USA.
[Irwin, G. M.; Qiu, X.; Wojcicki, S. G.] Stanford Univ, Dept Phys, Stanford, CA 94305 USA.
[Devenish, N. E.; Falk, E.; Hartnell, J.] Univ Sussex, Dept Phys & Astron, Brighton BN1 9QH, E Sussex, England.
[Webb, R. C.] Texas A&M Univ, Dept Phys, College Stn, TX 77843 USA.
[Cao, S. V.; Carroll, T. J.; De Rijck, S.; Flanagan, W.; Huang, J.; Lang, K.; Mehdiyev, R.; Phan, D. D.; Sail, P.; Schreckenberger, A.] Univ Texas Austin, Dept Phys, Austin, TX 78712 USA.
[Coelho, J. A. B.; Gallagher, H. R.; Kafka, T.; Mann, W. A.; Mayer, N.; Schneps, J.] Tufts Univ, Dept Phys, Medford, MA 02155 USA.
[Grzelak, K.] Univ Warsaw, Dept Phys, PL-02093 Warsaw, Poland.
[Devan, A. V.; Kordosky, M.; Nelson, J. K.; Radovic, A.; Vahle, P.] Coll William & Mary, Dept Phys, Williamsburg, VA 23187 USA.
RP Adamson, P (reprint author), Fermilab Natl Accelerator Lab, Batavia, IL 60510 USA.
RI Ling, Jiajie/I-9173-2014; Gomes, Ricardo/B-6899-2008;
OI Ling, Jiajie/0000-0003-2982-0670; Gomes, Ricardo/0000-0003-0278-4876;
Hartnell, Jeffrey/0000-0002-1744-7955; Castromonte Flores, Cesar
Manuel/0000-0002-9559-3704; Weber, Alfons/0000-0002-8222-6681
FU U.S. DOE; U.K. STFC; U.S. NSF; State and University of Minnesota; Brazil
FAPESP; Brazil CNPq; Brazil CAPES
FX This work was supported by the U.S. DOE, the U.K. STFC, the U.S. NSF,
the State and University of Minnesota, and Brazil's FAPESP, CNPq and
CAPES. We are grateful to the Minnesota Department of Natural Resources
and the personnel of the Soudan Laboratory and Fermilab. We thank the
Texas Advanced Computing Center at The University of Texas at Austin for
the provision of computing resources. We thank A. Smirnov and C. Giunti
for useful discussions.
NR 42
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PU AMER PHYSICAL SOC
PI COLLEGE PK
PA ONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA
SN 0031-9007
EI 1079-7114
J9 PHYS REV LETT
JI Phys. Rev. Lett.
PD OCT 7
PY 2016
VL 117
IS 15
AR 151803
DI 10.1103/PhysRevLett.117.151803
PG 7
WC Physics, Multidisciplinary
SC Physics
GA DY7XF
UT WOS:000385341900008
PM 27768323
ER
PT J
AU An, FP
Balantekin, AB
Band, HR
Bishai, M
Blyth, S
Cao, D
Cao, GF
Cao, J
Cen, WR
Chan, YL
Chang, JF
Chang, LC
Chang, Y
Chen, HS
Chen, QY
Chen, SM
Chen, YX
Chen, Y
Cheng, JH
Cheng, J
Cheng, YP
Cheng, ZK
Cherwinka, JJ
Chu, MC
Chukanov, A
Cummings, JP
de Arcos, J
Deng, ZY
Ding, XF
Ding, YY
Diwan, MV
Dolgareva, M
Dove, J
Dwyer, DA
Edwards, WR
Gill, R
Gonchar, M
Gong, GH
Gong, H
Grassi, M
Gu, WQ
Guan, MY
Guo, L
Guo, RP
Guo, XH
Guo, Z
Hackenburg, RW
Han, R
Hans, S
He, M
Heeger, KM
Heng, YK
Higuera, A
Hor, YK
Hsiung, YB
Hu, BZ
Hu, T
Hu, W
Huang, EC
Huang, HX
Huang, XT
Huber, P
Huo, W
Hussain, G
Jaffe, DE
Jaffke, P
Jen, KL
Jetter, S
Ji, XP
Ji, XL
Jiao, JB
Johnson, RA
Joshi, J
Kang, L
Kettell, SH
Kohn, S
Kramer, M
Kwan, KK
Kwok, MW
Kwok, T
Langford, TJ
Lau, K
Lebanowski, L
Lee, J
Lee, JHC
Lei, RT
Leitner, R
Leung, JKC
Li, C
Li, DJ
Li, F
Li, GS
Li, QJ
Li, S
Li, SC
Li, WD
Li, XN
Li, YF
Li, ZB
Liang, H
Lin, CJ
Lin, GL
Lin, S
Lin, SK
Lin, YC
Ling, JJ
Link, JM
Littenberg, L
Littlejohn, BR
Liu, DW
Liu, JL
Liu, JC
Loh, CW
Lu, C
Lu, HQ
Lu, JS
Luk, KB
Lv, Z
Ma, QM
Ma, XY
Ma, XB
Ma, YQ
Malyshkin, Y
Caicedo, DAM
McDonald, KT
McKeown, RD
Mitchell, I
Mooney, M
Nakajima, Y
Napolitano, J
Naumov, D
Naumova, E
Ngai, HY
Ning, Z
Ochoa-Ricoux, JP
Olshevskiy, A
Pan, HR
Park, J
Patton, S
Pec, V
Peng, JC
Pinsky, L
Pun, CSJ
Qi, FZ
Qi, M
Qian, X
Raper, N
Ren, J
Rosero, R
Roskovec, B
Ruan, XC
Steiner, H
Sun, GX
Sun, JL
Tang, W
Taychenachev, D
Treskov, K
Tsang, KV
Tull, CE
Viaux, N
Viren, B
Vorobel, V
Wang, CH
Wang, M
Wang, NY
Wang, RG
Wang, W
Wang, X
Wang, YF
Wang, Z
Wang, Z
Wang, ZM
Wei, HY
Wen, LJ
Whisnant, K
White, CG
Whitehead, L
Wise, T
Wong, HLH
Wong, SCF
Worcester, E
Wu, CH
Wu, Q
Wu, WJ
Xia, DM
Xia, JK
Xing, ZZ
Xu, JY
Xu, JL
Xu, Y
Xue, T
Yang, CG
Yang, H
Yang, L
Yang, MS
Yang, MT
Ye, M
Ye, Z
Yeh, M
Young, BL
Yu, ZY
Zeng, S
Zhan, L
Zhang, C
Zhang, HH
Zhang, JW
Zhang, QM
Zhang, XT
Zhang, YM
Zhang, YX
Zhang, YM
Zhang, ZJ
Zhang, ZY
Zhang, ZP
Zhao, J
Zhao, QW
Zhao, YB
Zhong, WL
Zhou, L
Zhou, N
Zhuang, HL
Zou, JH
AF An, F. P.
Balantekin, A. B.
Band, H. R.
Bishai, M.
Blyth, S.
Cao, D.
Cao, G. F.
Cao, J.
Cen, W. R.
Chan, Y. L.
Chang, J. F.
Chang, L. C.
Chang, Y.
Chen, H. S.
Chen, Q. Y.
Chen, S. M.
Chen, Y. X.
Chen, Y.
Cheng, J. -H.
Cheng, J.
Cheng, Y. P.
Cheng, Z. K.
Cherwinka, J. J.
Chu, M. C.
Chukanov, A.
Cummings, J. P.
de Arcos, J.
Deng, Z. Y.
Ding, X. F.
Ding, Y. Y.
Diwan, M. V.
Dolgareva, M.
Dove, J.
Dwyer, D. A.
Edwards, W. R.
Gill, R.
Gonchar, M.
Gong, G. H.
Gong, H.
Grassi, M.
Gu, W. Q.
Guan, M. Y.
Guo, L.
Guo, R. P.
Guo, X. H.
Guo, Z.
Hackenburg, R. W.
Han, R.
Hans, S.
He, M.
Heeger, K. M.
Heng, Y. K.
Higuera, A.
Hor, Y. K.
Hsiung, Y. B.
Hu, B. Z.
Hu, T.
Hu, W.
Huang, E. C.
Huang, H. X.
Huang, X. T.
Huber, P.
Huo, W.
Hussain, G.
Jaffe, D. E.
Jaffke, P.
Jen, K. L.
Jetter, S.
Ji, X. P.
Ji, X. L.
Jiao, J. B.
Johnson, R. A.
Joshi, J.
Kang, L.
Kettell, S. H.
Kohn, S.
Kramer, M.
Kwan, K. K.
Kwok, M. W.
Kwok, T.
Langford, T. J.
Lau, K.
Lebanowski, L.
Lee, J.
Lee, J. H. C.
Lei, R. T.
Leitner, R.
Leung, J. K. C.
Li, C.
Li, D. J.
Li, F.
Li, G. S.
Li, Q. J.
Li, S.
Li, S. C.
Li, W. D.
Li, X. N.
Li, Y. F.
Li, Z. B.
Liang, H.
Lin, C. J.
Lin, G. L.
Lin, S.
Lin, S. K.
Lin, Y. -C.
Ling, J. J.
Link, J. M.
Littenberg, L.
Littlejohn, B. R.
Liu, D. W.
Liu, J. L.
Liu, J. C.
Loh, C. W.
Lu, C.
Lu, H. Q.
Lu, J. S.
Luk, K. B.
Lv, Z.
Ma, Q. M.
Ma, X. Y.
Ma, X. B.
Ma, Y. Q.
Malyshkin, Y.
Caicedo, D. A. Martinez
McDonald, K. T.
McKeown, R. D.
Mitchell, I.
Mooney, M.
Nakajima, Y.
Napolitano, J.
Naumov, D.
Naumova, E.
Ngai, H. Y.
Ning, Z.
Ochoa-Ricoux, J. P.
Olshevskiy, A.
Pan, H. -R.
Park, J.
Patton, S.
Pec, V.
Peng, J. C.
Pinsky, L.
Pun, C. S. J.
Qi, F. Z.
Qi, M.
Qian, X.
Raper, N.
Ren, J.
Rosero, R.
Roskovec, B.
Ruan, X. C.
Steiner, H.
Sun, G. X.
Sun, J. L.
Tang, W.
Taychenachev, D.
Treskov, K.
Tsang, K. V.
Tull, C. E.
Viaux, N.
Viren, B.
Vorobel, V.
Wang, C. H.
Wang, M.
Wang, N. Y.
Wang, R. G.
Wang, W.
Wang, X.
Wang, Y. F.
Wang, Z.
Wang, Z.
Wang, Z. M.
Wei, H. Y.
Wen, L. J.
Whisnant, K.
White, C. G.
Whitehead, L.
Wise, T.
Wong, H. L. H.
Wong, S. C. F.
Worcester, E.
Wu, C. -H.
Wu, Q.
Wu, W. J.
Xia, D. M.
Xia, J. K.
Xing, Z. Z.
Xu, J. Y.
Xu, J. L.
Xu, Y.
Xue, T.
Yang, C. G.
Yang, H.
Yang, L.
Yang, M. S.
Yang, M. T.
Ye, M.
Ye, Z.
Yeh, M.
Young, B. L.
Yu, Z. Y.
Zeng, S.
Zhan, L.
Zhang, C.
Zhang, H. H.
Zhang, J. W.
Zhang, Q. M.
Zhang, X. T.
Zhang, Y. M.
Zhang, Y. X.
Zhang, Y. M.
Zhang, Z. J.
Zhang, Z. Y.
Zhang, Z. P.
Zhao, J.
Zhao, Q. W.
Zhao, Y. B.
Zhong, W. L.
Zhou, L.
Zhou, N.
Zhuang, H. L.
Zou, J. H.
CA Daya Bay Collaboration
TI Improved Search for a Light Sterile Neutrino with the Full Configuration
of the Daya Bay Experiment
SO PHYSICAL REVIEW LETTERS
LA English
DT Article
ID ANTINEUTRINO DETECTORS; SYSTEM
AB This Letter reports an improved search for light sterile neutrino mixing in the electron antineutrino disappearance channel with the full configuration of the Daya Bay Reactor Neutrino Experiment. With an additional 404 days of data collected in eight antineutrino detectors, this search benefits from 3.6 times the statistics available to the previous publication, as well as from improvements in energy calibration and background reduction. A relative comparison of the rate and energy spectrum of reactor antineutrinos in the three experimental halls yields no evidence of sterile neutrino mixing in the 2 x 10(-4) less than or similar to vertical bar Delta m(41)(2)vertical bar less than or similar to 0.3 eV(2) mass range. The resulting limits on sin(2) 2 theta(14) are improved by approx imately a factor of 2 over previous results and constitute the most stringent constraints to date in the vertical bar Delta m(41)(2)vertical bar less than or similar to 0.2 eV(2) region.
C1 [An, F. P.] East China Univ Sci & Technol, Inst Modern Phys, Shanghai, Peoples R China.
[Balantekin, A. B.; Cherwinka, J. J.; Wise, T.] Univ Wisconsin, Madison, WI USA.
[Band, H. R.; Heeger, K. M.; Langford, T. J.] Yale Univ, Dept Phys, New Haven, CT USA.
[Bishai, M.; Diwan, M. V.; Gill, R.; Hackenburg, R. W.; Hans, S.; Jaffe, D. E.; Joshi, J.; Kettell, S. H.; Littenberg, L.; Mooney, M.; Qian, X.; Rosero, R.; Tang, W.; Viren, B.; Worcester, E.; Yeh, M.; Zhang, C.] Brookhaven Natl Lab, Upton, NY 11973 USA.
[Blyth, S.; Hsiung, Y. B.; Hu, B. Z.; Lin, Y. -C.; Pan, H. -R.] Natl Taiwan Univ, Dept Phys, Taipei, Taiwan.
[Blyth, S.; Chang, Y.; Wang, C. H.] Natl United Univ, Miaoli, Taiwan.
[Cao, D.; Loh, C. W.; Qi, M.; Yang, H.] Nanjing Univ, Nanjing, Jiangsu, Peoples R China.
[Cao, G. F.; Cao, J.; Cen, W. R.; Chang, J. F.; Chen, H. S.; Cheng, Y. P.; Deng, Z. Y.; Ding, X. F.; Ding, Y. Y.; Grassi, M.; Guan, M. Y.; Guo, R. P.; He, M.; Heng, Y. K.; Hu, T.; Hu, W.; Jetter, S.; Ji, X. L.; Li, F.; Li, Q. J.; Li, W. D.; Li, X. N.; Li, Y. F.; Liu, J. C.; Lu, H. Q.; Lu, J. S.; Ma, Q. M.; Ma, X. Y.; Ma, Y. Q.; Ning, Z.; Qi, F. Z.; Sun, G. X.; Wang, R. G.; Wang, Y. F.; Wang, Z.; Wang, Z. M.; Wen, L. J.; Wu, W. J.; Xia, J. K.; Xing, Z. Z.; Xu, J. L.; Yang, C. G.; Yang, M. S.; Ye, M.; Yu, Z. Y.; Zeng, S.; Zhan, L.; Zhang, J. W.; Zhang, X. T.; Zhang, Z. Y.; Zhao, J.; Zhao, Q. W.; Zhao, Y. B.; Zhong, W. L.; Zhou, L.; Zhuang, H. L.; Zou, J. H.] Inst High Energy Phys, Beijing, Peoples R China.
[Chan, Y. L.; Chu, M. C.; Kwan, K. K.; Kwok, M. W.; Xu, J. Y.] Chinese Univ Hong Kong, Hong Kong, Hong Kong, Peoples R China.
[Chang, L. C.; Cheng, J. -H.; Jen, K. L.; Lin, G. L.; Wu, C. -H.] Natl Chiao Tung Univ, Inst Phys, Hsinchu, Taiwan.
[Chen, Q. Y.; Cheng, J.; Huang, X. T.; Jiao, J. B.; Li, C.; Wang, M.; Wu, Q.; Yang, M. T.] Shandong Univ, Jinan, Peoples R China.
[Chen, S. M.; Gong, G. H.; Gong, H.; Guo, L.; Guo, Z.; Hussain, G.; Ji, X. P.; Lebanowski, L.; Wang, Z.; Wei, H. Y.; Zhang, Y. M.] Tsinghua Univ, Dept Engn Phys, Beijing, Peoples R China.
[Chen, Y. X.; Han, R.; Ma, X. B.] North China Elect Power Univ, Beijing, Peoples R China.
[Chen, Y.] Shenzhen Univ, Shenzhen, Peoples R China.
[Cheng, Z. K.; Li, Z. B.; Ling, J. J.; Wang, W.; Wong, S. C. F.; Xu, Y.; Xue, T.; Zhang, H. H.; Zhang, Y. M.] Sun Yat Sen Zhongshan Univ, Guangzhou, Guangdong, Peoples R China.
[Chukanov, A.; Dolgareva, M.; Gonchar, M.; Naumov, D.; Naumova, E.; Olshevskiy, A.; Taychenachev, D.; Treskov, K.] Joint Inst Nucl Res, Dubna, Moscow Region, Russia.
[Cummings, J. P.] Siena Coll, Loudonville, NY USA.
[de Arcos, J.; Littlejohn, B. R.; Caicedo, D. A. Martinez; White, C. G.] IIT, Dept Phys, Chicago, IL USA.
[Dove, J.; Huang, E. C.; Peng, J. C.] Univ Illinois, Dept Phys, Urbana, IL USA.
[Dwyer, D. A.; Edwards, W. R.; Kramer, M.; Lee, J.; Lin, C. J.; Luk, K. B.; Nakajima, Y.; Patton, S.; Steiner, H.; Tsang, K. V.; Tull, C. E.; Wong, H. L. H.] Lawrence Berkeley Natl Lab, Berkeley, CA USA.
[Gu, W. Q.; Li, G. S.; Liu, J. L.] Shanghai Jiao Tong Univ, Dept Phys & Astron, Shanghai Lab Particle Phys & Cosmol, Shanghai, Peoples R China.
[Guo, X. H.; Wang, N. Y.] Beijing Normal Univ, Beijing, Peoples R China.
[Higuera, A.; Lau, K.; Lin, S. K.; Liu, D. W.; Mitchell, I.; Pinsky, L.; Whitehead, L.; Ye, Z.] Univ Houston, Dept Phys, Houston, TX USA.
[Hor, Y. K.; Huber, P.; Jaffke, P.; Li, S. C.; Link, J. M.; Park, J.] Virginia Tech, Ctr Neutrino Phys, Blacksburg, VA USA.
[Huang, H. X.; Ren, J.; Ruan, X. C.] China Inst Atom Energy, Beijing, Peoples R China.
[Huo, W.; Li, D. J.; Liang, H.; Zhang, Z. P.; Zhou, N.] Univ Sci & Technol China, Hefei, Peoples R China.
[Ji, X. P.] Nankai Univ, Sch Phys, Tianjin, Peoples R China.
[Johnson, R. A.] Univ Cincinnati, Dept Phys, Cincinnati, OH USA.
[Kang, L.; Lei, R. T.; Li, S.; Lin, S.; Yang, L.; Zhang, Z. J.] Dongguan Univ Technol, Dongguan, Peoples R China.
[Kohn, S.; Kramer, M.; Luk, K. B.; Steiner, H.; Wong, H. L. H.] Univ Calif Berkeley, Dept Phys, Berkeley, CA 94720 USA.
[Kwok, T.; Lee, J. H. C.; Leung, J. K. C.; Li, S. C.; Ngai, H. Y.; Pun, C. S. J.] Univ Hong Kong, Dept Phys, Pokfulam, Hong Kong, Peoples R China.
[Leitner, R.; Pec, V.; Roskovec, B.; Vorobel, V.] Charles Univ Prague, Fac Math & Phys, Prague, Czech Republic.
[Lu, C.; McDonald, K. T.] Princeton Univ, Joseph Henry Labs, Princeton, NJ 08544 USA.
[Lv, Z.; Zhang, Q. M.] Xi An Jiao Tong Univ, Xian, Peoples R China.
[Malyshkin, Y.; Ochoa-Ricoux, J. P.; Viaux, N.] Pontificia Univ Catolica Chile, Inst Fis, Santiago, Chile.
[McKeown, R. D.] CALTECH, Pasadena, CA 91125 USA.
[McKeown, R. D.; Wang, W.] Coll William & Mary, Williamsburg, VA USA.
[Napolitano, J.] Temple Univ, Coll Sci & Technol, Dept Phys, Philadelphia, PA 19122 USA.
[Raper, N.] Rensselaer Polytech Inst, Dept Phys Appl Phys & Astron, Troy, NY USA.
[Sun, J. L.; Zhang, Y. X.] China Gen Nucl Power Grp, Shenzhen, Peoples R China.
[Wang, X.] Natl Univ Def Technol, Coll Elect Sci & Engn, Changsha, Hunan, Peoples R China.
[Young, B. L.] Iowa State Univ, Ames, IA USA.
[Xia, D. M.] Chongqing Univ, Chongqing, Peoples R China.
RP An, FP (reprint author), East China Univ Sci & Technol, Inst Modern Phys, Shanghai, Peoples R China.
RI Ling, Jiajie/I-9173-2014; Leitner, Rupert/C-2004-2017; Liu,
Jianglai/P-2587-2015;
OI Ling, Jiajie/0000-0003-2982-0670; Leitner, Rupert/0000-0002-2994-2187;
Liu, Jianglai/0000-0002-4563-3157; Qian, Xin/0000-0002-7903-7935; Zhang,
Chao/0000-0003-2298-6272; Grassi, Marco/0000-0003-2422-6736; Gonchar,
Maxim/0000-0002-6820-9471
FU Ministry of Science and Technology of China; U.S. Department of Energy;
Chinese Academy of Sciences (CAS); CAS Center for Excellence in Particle
Physics; National Natural Science Foundation of China; Guangdong
provincial government; Shenzhen municipal government; China General
Nuclear Power Group; Laboratory Directed Research and Development
Program of the Institute of High Energy Physics; Shanghai Laboratory for
Particle Physics and Cosmology; Research Grants Council of the Hong Kong
Special Administrative Region of China; University Development Fund of
the University of Hong Kong; MOE program for Research of Excellence at
National Taiwan University; National Chiao-Tung University; MOST from
Taiwan; U.S. National Science Foundation; Alfred P. Sloan Foundation;
Laboratory Directed Research and Development Program of Berkeley
National Laboratory; Ministry of Education, Youth, and Sports of the
Czech Republic; Joint Institute of Nuclear Research in Dubna, Russia;
NSFC-RFBR joint research program; National Commission for Scientific and
Technology Research of Chile; Laboratory Directed Research and
Development Program of Brookhaven National Laboratory; Charles
University in Prague
FX The Daya Bay Reactor Neutrino Experiment is supported in part by the
Ministry of Science and Technology of China, the U.S. Department of
Energy, the Chinese Academy of Sciences (CAS), the CAS Center for
Excellence in Particle Physics, the National Natural Science Foundation
of China, the Guangdong provincial government, the Shenzhen municipal
government, the China General Nuclear Power Group, the Laboratory
Directed Research and Development Program of the Institute of High
Energy Physics, the Shanghai Laboratory for Particle Physics and
Cosmology, the Research Grants Council of the Hong Kong Special
Administrative Region of China, the University Development Fund of the
University of Hong Kong, the MOE program for Research of Excellence at
National Taiwan University, National Chiao-Tung University, MOST funding
support from Taiwan, the U.S. National Science Foundation, the Alfred P.
Sloan Foundation, the Laboratory Directed Research and Development
Program of Berkeley National Laboratory and Brookhaven National
Laboratory, the Ministry of Education, Youth, and Sports of the Czech
Republic, Charles University in Prague, the Joint Institute of Nuclear
Research in Dubna, Russia, the NSFC-RFBR joint research program, and the
National Commission for Scientific and Technology Research of Chile. We
acknowledge the Yellow River Engineering Consulting Co., Ltd., and the
China Railway 15th Bureau Group Co., Ltd., for building the underground
laboratory. We are grateful for the ongoing cooperation from the China
General Nuclear Power Group and China Light and Power Company.
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PI COLLEGE PK
PA ONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA
SN 0031-9007
EI 1079-7114
J9 PHYS REV LETT
JI Phys. Rev. Lett.
PD OCT 7
PY 2016
VL 117
IS 15
AR 151802
DI 10.1103/PhysRevLett.117.151802
PG 7
WC Physics, Multidisciplinary
SC Physics
GA DY7XF
UT WOS:000385341900007
PM 27768341
ER
PT J
AU Dornheim, T
Groth, S
Sjostrom, T
Malone, FD
Foulkes, WMC
Bonitz, M
AF Dornheim, Tobias
Groth, Simon
Sjostrom, Travis
Malone, Fionn D.
Foulkes, W. M. C.
Bonitz, Michael
TI Ab Initio Quantum Monte Carlo Simulation of the Warm Dense Electron Gas
in the Thermodynamic Limit
SO PHYSICAL REVIEW LETTERS
LA English
DT Article
ID FINITE TEMPERATURES; GROUND-STATE; SYSTEMS; PLASMAS; EXCHANGE; MATTER
AB We perform ab initio quantum Monte Carlo (QMC) simulations of the warm dense uniform electron gas in the thermodynamic limit. By combining QMC data with the linear response theory, we are able to remove finite-size errors from the potential energy over the substantial parts of the warm dense regime, overcoming the deficiencies of the existing finite-size corrections by Brown et al. [Phys. Rev. Lett. 110, 146405 (2013)]. Extensive new QMC results for up to N = 1000 electrons enable us to compute the potential energy V and the exchange-correlation free energy F-xc of the macroscopic electron gas with an unprecedented accuracy of vertical bar Delta V vertical bar/vertical bar V vertical bar,vertical bar Delta F-xc vertical bar/similar to 10(-3). A comparison of our new data to the recent parametrization of F-xc by Karasiev et al. [Phys. Rev. Lett. 112, 076403 (2014)] reveals significant deviations to the latter.
C1 [Dornheim, Tobias; Groth, Simon; Bonitz, Michael] Univ Kiel, Inst Theoret Phys & Astrophys, D-24098 Kiel, Germany.
[Sjostrom, Travis] Los Alamos Natl Lab, Div Theoret, Los Alamos, NM 87545 USA.
[Malone, Fionn D.; Foulkes, W. M. C.] Imperial Coll London, Dept Phys, Exhibit Rd, London SW7 2AZ, England.
RP Dornheim, T (reprint author), Univ Kiel, Inst Theoret Phys & Astrophys, D-24098 Kiel, Germany.
EM dornheim@theo-physik.uni-kiel.de
RI Bonitz, Michael/A-6873-2010;
OI Bonitz, Michael/0000-0001-7911-0656; Foulkes,
Matthew/0000-0001-8359-1122
FU Deutsche Forschungsgemeinschaft [BO1366-10, SFB TR-24, A9];
Norddeutscher Verbund fur Hoch- und Hochstleistungsrechnen (HLRN)
[shp00015]; U.S. DOE/NNSA [DE-AC52-06NA25396]; Imperial College Ph.D.
Scholarship; Swiss National Supercomputing Centre (CSCS) [s523]; ARCHER;
United Kingdom National Supercomputing Service; EPSRC [EP/K038141/1];
RAP award; Thomas Young Centre [TYC-101]
FX We acknowledge stimulating discussions with Tim Schoof and Jim Dufty and
are grateful to Jan Vorberger for providing the Montroll-Ward and
e4 data shown in Fig. 1. This work was supported by the
Deutsche Forschungsgemeinschaft via Project No. BO1366-10 and via SFB
TR-24 Project No. A9 as well as Grant No. shp00015 for CPU time at the
Norddeutscher Verbund fur Hoch- und Hochstleistungsrechnen (HLRN). T. S.
acknowledges the support of the U.S. DOE/NNSA under Contract No.
DE-AC52-06NA25396. F. D. M. is funded by an Imperial College Ph.D.
Scholarship. F. D. M. and W. M. C. F. used computing facilities provided
by the High Performance Computing Service of Imperial College London, by
the Swiss National Supercomputing Centre (CSCS) under Project ID No.
s523, and by ARCHER, the United Kingdom National Supercomputing Service,
under EPSRC Grant No. EP/K038141/1 and via a RAP award. F. D. M. and W.
M. C. F. acknowledge the research environment provided by the Thomas
Young Centre under Grant No. TYC-101.
NR 52
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PU AMER PHYSICAL SOC
PI COLLEGE PK
PA ONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA
SN 0031-9007
EI 1079-7114
J9 PHYS REV LETT
JI Phys. Rev. Lett.
PD OCT 7
PY 2016
VL 117
IS 15
AR 156403
DI 10.1103/PhysRevLett.117.156403
PG 6
WC Physics, Multidisciplinary
SC Physics
GA DY7XF
UT WOS:000385341900021
PM 27768371
ER
PT J
AU Heres, M
Wang, Y
Griffin, PJ
Gainaru, C
Sokolov, AP
AF Heres, M.
Wang, Y.
Griffin, P. J.
Gainaru, C.
Sokolov, A. P.
TI Proton Conductivity in Phosphoric Acid: The Role of Quantum Effects
SO PHYSICAL REVIEW LETTERS
LA English
DT Article
ID GLASS-TRANSITION; ION CONDUCTION; EXCESS PROTON; HYDROGEN-BOND;
FUEL-CELLS; WATER; DYNAMICS; MECHANISM; TRANSPORT
AB Phosphoric acid has one of the highest intrinsic proton conductivities of any known liquids, and the mechanism of this exceptional conductivity remains a puzzle. Our detailed experimental studies discovered a strong isotope effect in the conductivity of phosphoric acids caused by (i) a strong isotope shift of the glass transition temperature and (ii) a significant reduction of the energy barrier by zero-point quantum fluctuations. These results suggest that the high conductivity in phosphoric acids is caused by a very efficient proton transfer mechanism, which is strongly assisted by quantum effects.
C1 [Heres, M.] Univ Tennessee, Dept Chem & Biomol Engn, Knoxville, TN 37996 USA.
[Wang, Y.] Oak Ridge Natl Lab, Ctr Nanophase Mat Sci, Oak Ridge, TN 37831 USA.
[Griffin, P. J.] Univ Penn, Dept Mat Sci & Engn, Philadelphia, PA 19104 USA.
[Gainaru, C.; Sokolov, A. P.] Univ Tennessee, Dept Chem, Knoxville, TN 37996 USA.
[Sokolov, A. P.] Oak Ridge Natl Lab, Div Chem Sci, Oak Ridge, TN 37831 USA.
RP Sokolov, AP (reprint author), Univ Tennessee, Dept Chem, Knoxville, TN 37996 USA.; Sokolov, AP (reprint author), Oak Ridge Natl Lab, Div Chem Sci, Oak Ridge, TN 37831 USA.
EM sokolov@utk.edu
FU NSF Chemistry Program [CHE-1213444]
FX We greatly acknowledge support from the NSF Chemistry Program under
Grant No. CHE-1213444.
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PU AMER PHYSICAL SOC
PI COLLEGE PK
PA ONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA
SN 0031-9007
EI 1079-7114
J9 PHYS REV LETT
JI Phys. Rev. Lett.
PD OCT 7
PY 2016
VL 117
IS 15
AR 156001
DI 10.1103/PhysRevLett.117.156001
PG 5
WC Physics, Multidisciplinary
SC Physics
GA DY7XF
UT WOS:000385341900019
PM 27768354
ER
PT J
AU Rupp, D
Fluckiger, L
Adolph, M
Gorkhover, T
Krikunova, M
Muller, JP
Muller, M
Oelze, T
Ovcharenko, Y
Roben, B
Sauppe, M
Schorb, S
Wolter, D
Mitzner, R
Wostmann, M
Roling, S
Harmand, M
Treusch, R
Arbeiter, M
Fennel, T
Bostedt, C
Moller, T
AF Rupp, Daniela
Flueckiger, Leonie
Adolph, Marcus
Gorkhover, Tais
Krikunova, Maria
Mueller, Jan Philippe
Mueller, Maria
Oelze, Tim
Ovcharenko, Yevheniy
Roeben, Benjamin
Sauppe, Mario
Schorb, Sebastian
Wolter, David
Mitzner, Rolf
Wostmann, Michael
Roling, Sebastian
Harmand, Marion
Treusch, Rolf
Arbeiter, Mathias
Fennel, Thomas
Bostedt, Christoph
Moeller, Thomas
TI Recombination-Enhanced Surface Expansion of Clusters in Intense Soft
X-Ray Laser Pulses
SO PHYSICAL REVIEW LETTERS
LA English
DT Article
ID FREE-ELECTRON LASER; MULTIPLE IONIZATION; MASS-SPECTROMETRY;
FEMTOSECOND; DYNAMICS; ENERGY; NANOPARTICLES; EXPLOSIONS; BEAMS
AB We studied the nanoplasma formation and explosion dynamics of single large xenon clusters in ultrashort, intense x-ray free-electron laser pulses via ion spectroscopy. The simultaneous measurement of single-shot diffraction images enabled a single-cluster analysis that is free from any averaging over the cluster size and laser intensity distributions. The measured charge state-resolved ion energy spectra show narrow distributions with peak positions that scale linearly with final ion charge state. These two distinct signatures are attributed to highly efficient recombination that eventually leads to the dominant formation of neutral atoms in the cluster. The measured mean ion energies exceed the value expected without recombination by more than an order of magnitude, indicating that the energy release resulting from electron-ion recombination constitutes a previously unnoticed nanoplasma heating process. This conclusion is supported by results from semiclassical molecular dynamics simulations.
C1 [Rupp, Daniela; Flueckiger, Leonie; Adolph, Marcus; Gorkhover, Tais; Krikunova, Maria; Mueller, Jan Philippe; Mueller, Maria; Oelze, Tim; Ovcharenko, Yevheniy; Roeben, Benjamin; Sauppe, Mario; Schorb, Sebastian; Wolter, David; Moeller, Thomas] Tech Univ Berlin, IOAP, Hardenbergstr 36, D-10623 Berlin, Germany.
[Flueckiger, Leonie] La Trobe Univ, ARC Ctr Excellence Adv Mol Imaging, Bundoora, Vic 3086, Australia.
[Gorkhover, Tais; Schorb, Sebastian; Bostedt, Christoph] SLAC, LCLS, 2575 Sand Hill Rd, Menlo Pk, CA 94025 USA.
[Mitzner, Rolf] Helmholtz Zentrum Berlin, Hahn Meitner Pl 1, D-14109 Berlin, Germany.
[Wostmann, Michael; Roling, Sebastian] Univ Munster, Wilhelm Klemm Str 10, D-48149 Munster, Germany.
[Harmand, Marion; Treusch, Rolf] DESY, FLASH, Notkestr 85, D-22603 Hamburg, Germany.
[Arbeiter, Mathias; Fennel, Thomas] Univ Rostock, Inst Phys, Albert Einstein Str 23, D-18059 Rostock, Germany.
[Bostedt, Christoph] Argonne Natl Lab, 9700 S Cass Ave, Argonne, IL 60439 USA.
[Bostedt, Christoph] Northwestern Univ, Dept Phys & Astron, 2145 Sheridan Rd, Evanston, IL 60208 USA.
RP Rupp, D (reprint author), Tech Univ Berlin, IOAP, Hardenbergstr 36, D-10623 Berlin, Germany.
EM daniela.rupp@physik.tu-berlin.de; thomas.fennel@uni-rostock.de
RI Rupp, Daniela/P-7590-2016; harmand, marion/Q-1248-2016
OI harmand, marion/0000-0003-0713-5824
FU IOAP; DESY; BMBF [05K10KT2, 05K13KT2]; DFG [BO 3169/2-2, MO 719/13-1,
SFB 652/3]; U.S. Department of Energy, Office of Basic Energy Sciences,
Division of Chemical, Geological, and Biological Sciences
[DE-AC02-06CH11357]
FX Excellent support from IOAP and DESY workshops is acknowledged. The
experiments have been funded by BMBF Grants No. 05K10KT2 and No.
05K13KT2 (FSP FLASH) and DFG Grants No. BO 3169/2-2 and No. MO 719/13-1.
T.F. acknowledges financial support by the DFG within SFB 652/3 and
computer time provided by the North German Supercomputing Alliance
(HLRN). C. B. acknowledges support from the U.S. Department of Energy,
Office of Basic Energy Sciences, Division of Chemical, Geological, and
Biological Sciences, under Contract No. DE-AC02-06CH11357.
NR 55
TC 0
Z9 0
U1 12
U2 12
PU AMER PHYSICAL SOC
PI COLLEGE PK
PA ONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA
SN 0031-9007
EI 1079-7114
J9 PHYS REV LETT
JI Phys. Rev. Lett.
PD OCT 7
PY 2016
VL 117
IS 15
DI 10.1103/PhysRevLett.117.153401
PG 6
WC Physics, Multidisciplinary
SC Physics
GA DY7XF
UT WOS:000385341900011
PM 27768378
ER
PT J
AU Hirsh, DA
Rossini, AJ
Emsley, L
Schurko, RW
AF Hirsh, David A.
Rossini, Aaron J.
Emsley, Lyndon
Schurko, Robert W.
TI Cl-35 dynamic nuclear polarization solid-state NMR of active
pharmaceutical ingredients
SO PHYSICAL CHEMISTRY CHEMICAL PHYSICS
LA English
DT Article
ID AMPLITUDE CROSS-POLARIZATION; INTEGER QUADRUPOLAR NUCLEI; METAL-ORGANIC
FRAMEWORKS; ANGLE-SPINNING NMR; MAS NMR; CORRELATION SPECTROSCOPY;
MAGNETIC-RESONANCE; ADIABATIC PULSES; CHEMICAL-SHIFTS; HIGH-FREQUENCY
AB In this work, we show how to obtain efficient dynamic nuclear polarization (DNP) enhanced Cl-35 solid-state NMR (SSNMR) spectra at 9.4 T and demonstrate how they can be used to characterize the molecular-level structure of hydrochloride salts of active pharmaceutical ingredients (APIs) in both bulk and low wt% API dosage forms. Cl-35 SSNMR central-transition powder patterns of chloride ions are typically tens to hundreds of kHz in breadth, and most cannot be excited uniformly with high-power rectangular pulses or acquired under conditions of magic-angle spinning (MAS). Herein, we demonstrate the combination of DNP and H-1-Cl-35 broadband adiabatic inversion cross polarization (BRAIN-CP) experiments for the acquisition of high quality wideline spectra of APIs under static sample conditions, and obtain signals up to 50 times greater than in spectra acquired without the use of DNP at 100 K. We report a new protocol, called spinning-on spinning-off (SOSO) acquisition, where MAS is applied during part of the polarization delay to increase the DNP enhancements and then the MAS rotation is stopped so that a wideline Cl-35 NMR powder pattern free from the effects of spinning sidebands can be acquired under static conditions. This method provides an additional two-fold signal enhancement compared to DNP-enhanced SSNMR spectra acquired under purely static conditions. DNP-enhanced Cl-35 experiments are used to characterize APIs in bulk and dosage forms with Cl contents as low as 0.45 wt%. These results are compared to DNP-enhanced H-1-C-13 CP/MAS spectra of APIs in dosage forms, which are often hindered by interfering signals arising from the binders, fillers and other excipient materials.
C1 [Hirsh, David A.; Schurko, Robert W.] Univ Windsor, Dept Chem & Biochem, Windsor, ON N9B 3P4, Canada.
[Rossini, Aaron J.] Iowa State Univ, Dept Chem, Ames, IA 50011 USA.
[Rossini, Aaron J.] US DOE, Ames Lab, Ames, IA 50011 USA.
[Emsley, Lyndon] Ecole Polytech Fed Lausanne, Inst Sci & Ingn Chim, CH-1015 Lausanne, Switzerland.
RP Schurko, RW (reprint author), Univ Windsor, Dept Chem & Biochem, Windsor, ON N9B 3P4, Canada.; Rossini, AJ (reprint author), Iowa State Univ, Dept Chem, Ames, IA 50011 USA.; Rossini, AJ (reprint author), US DOE, Ames Lab, Ames, IA 50011 USA.
EM arossini@iastate.edu; rschurko@uwindsor.ca
RI Emsley, Lyndon/C-6108-2008
OI Emsley, Lyndon/0000-0003-1360-2572
FU Natural Science and Engineering Research Council (NSERC, Canada);
Canadian Foundation for Innovation (CFI); Ontario Innovation Trust
(OIT); University of Windsor; US Department of Energy (DOE), Office of
Science, Basic Energy Sciences, Division of Materials Science and
Engineering and Division of Chemical Sciences, Geosciences, and
Biosciences; US DOE [DE-AC02-07CH11358]; Ames Laboratory (Royalty
Account); Iowa State University; ERC [320860]
FX R. W. S. acknowledges the Natural Science and Engineering Research
Council (NSERC, Canada) for support in the form of Discovery,
Accelerator, and Research Tools and Instruments (RTI) grants. He also
acknowledges the University of Windsor for a 50th Golden Jubilee
Research Chair. We are also grateful to the Canadian Foundation for
Innovation (CFI), the Ontario Innovation Trust (OIT), and the University
of Windsor for support of the Laboratories for Solid-State
Characterization. The DNP solid-state NMR spectrometer at the Ames
Laboratory was funded by US Department of Energy (DOE), Office of
Science, Basic Energy Sciences, Division of Materials Science and
Engineering and Division of Chemical Sciences, Geosciences, and
Biosciences. The Ames Laboratory is operated for the US DOE by Iowa
State University under contract no. DE-AC02-07CH11358. A. J. R. thanks
the Ames Laboratory (Royalty Account) and Iowa State University for
support. L. E. acknowledges the support of ERC Advanced Grant No.
320860. We thank Professors Holger Eichhorn and Jeremy Rawson (Windsor)
for their assistance with the VT-pXRD measurements. We are grateful to
Prof. P. Tordo, Dr O. Ouari and Dr G. Casano (Aix-Marseille Universite,
France) for providing the TEKPol biradical used in the DNP experiments.
NR 106
TC 2
Z9 2
U1 26
U2 26
PU ROYAL SOC CHEMISTRY
PI CAMBRIDGE
PA THOMAS GRAHAM HOUSE, SCIENCE PARK, MILTON RD, CAMBRIDGE CB4 0WF, CAMBS,
ENGLAND
SN 1463-9076
EI 1463-9084
J9 PHYS CHEM CHEM PHYS
JI Phys. Chem. Chem. Phys.
PD OCT 7
PY 2016
VL 18
IS 37
BP 25893
EP 25904
DI 10.1039/c6cp04353d
PG 12
WC Chemistry, Physical; Physics, Atomic, Molecular & Chemical
SC Chemistry; Physics
GA DY5VN
UT WOS:000385172600015
PM 27711465
ER
PT J
AU Konstantinou, K
Sushko, PV
Duffy, DM
AF Konstantinou, Konstantinos
Sushko, Peter V.
Duffy, Dorothy M.
TI Modelling the local atomic structure of molybdenum in nuclear waste
glasses with ab initio molecular dynamics simulations
SO PHYSICAL CHEMISTRY CHEMICAL PHYSICS
LA English
DT Article
ID ALKALI BOROSILICATE GLASSES; LIME-SILICATE-GLASSES;
ELECTRONIC-PROPERTIES; MAS-NMR; SODIUM; LIQUID; EQUILIBRIUM; CERAMICS;
CRYSTALS; OXIDES
AB The nature of chemical bonding of molybdenum in high level nuclear waste glasses has been elucidated by ab initio molecular dynamics simulations. Two compositions, (SiO2)(57.5)-(B2O3)(10)-(Na2O)(15)-(CaO)(15)(MoO3)(2.5) and (SiO2)(57.3)-(B2O3)(20)-(Na2O)(6.8)-(Li2O)(13.4)-(MoO3)(2.5), were considered in order to investigate the effect of ionic and covalent components on the glass structure and the formation of the crystallisation precursors (Na2MoO4 and CaMoO4). The coordination environments of Mo cations and the corresponding bond lengths calculated from our model are in excellent agreement with experimental observations. The analysis of the first coordination shell reveals two different types of molybdenum host matrix bonds in the lithium sodium borosilicate glass. Based on the structural data and the bond valence model, we demonstrate that the Mo cation can be found in a redox state and the molybdate tetrahedron can be connected with the borosilicate network in a way that inhibits the formation of crystalline molybdates. These results significantly extend our understanding of bonding in Mo-containing nuclear waste glasses and demonstrate that tailoring the glass composition to specific heavy metal constituents can facilitate incorporation of heavy metals at high concentrations.
C1 [Konstantinou, Konstantinos; Duffy, Dorothy M.] UCL, Dept Phys & Astron, Gower St, London WC1E 6BT, England.
[Sushko, Peter V.] Pacific Northwest Natl Lab, Phys & Computat Sci Directorate, Div Phys Sci, Richland, WA 99352 USA.
RP Konstantinou, K (reprint author), UCL, Dept Phys & Astron, Gower St, London WC1E 6BT, England.
EM konstantinos.konstantinou.13@ucl.ac.uk
RI Sushko, Peter/F-5171-2013
OI Sushko, Peter/0000-0001-7338-4146
FU Impact Studentship scheme at UCL - IHI Corporation; UCL; Royal Society;
EPSRC [EP/L000202]
FX K. K. was supported through the Impact Studentship scheme at UCL
co-funded by the IHI Corporation and UCL. P. V. S. thanks the Royal
Society, which supported preliminary work on this project, and the
Laboratory Directed Research and Development program at PNNL, a
multiprogram national laboratory operated by Battelle for the U.S.
Department of Energy. Via our membership of the UK's HEC Materials
Chemistry Consortium, which is funded by EPSRC (EP/L000202), this work
used the ARCHER UK National Supercomputing Service
(http://www.archer.ac.uk).
NR 58
TC 0
Z9 0
U1 17
U2 17
PU ROYAL SOC CHEMISTRY
PI CAMBRIDGE
PA THOMAS GRAHAM HOUSE, SCIENCE PARK, MILTON RD, CAMBRIDGE CB4 0WF, CAMBS,
ENGLAND
SN 1463-9076
EI 1463-9084
J9 PHYS CHEM CHEM PHYS
JI Phys. Chem. Chem. Phys.
PD OCT 7
PY 2016
VL 18
IS 37
BP 26125
EP 26132
DI 10.1039/c6cp03076a
PG 8
WC Chemistry, Physical; Physics, Atomic, Molecular & Chemical
SC Chemistry; Physics
GA DY5VN
UT WOS:000385172600037
PM 27711386
ER
PT J
AU Kaspar, TC
Sushko, PV
Bowden, ME
Heald, SM
Papadogianni, A
Tschammer, C
Bierwagen, O
Chambers, SA
AF Kaspar, Tiffany C.
Sushko, Peter V.
Bowden, Mark E.
Heald, Steve M.
Papadogianni, Alexandra
Tschammer, Carsten
Bierwagen, Oliver
Chambers, Scott A.
TI Defect compensation by Cr vacancies and oxygen interstitials in Ti4+
-doped Cr2O3 epitaxial thin films
SO PHYSICAL REVIEW B
LA English
DT Article
ID MOLECULAR-BEAM EPITAXY; RAY PHOTOELECTRON-SPECTROSCOPY;
ELECTRICAL-CONDUCTIVITY; SURFACE-STRUCTURE; VAPOR-DEPOSITION; TIO2;
ALPHA-FE2O3; DIFFRACTION; DEPENDENCE; CHEMISTRY
AB Epitaxial thin films of Cr2-x TixO3 were deposited by oxygen-plasma-assisted molecular beam epitaxy for 0.04 <= x <= 0.26. Ti valence is verified by both x-ray photoelectron spectroscopy (XPS) and Ti K-edge x-ray absorption near-edge spectroscopy (XANES) to be Ti4+. Substitution of Ti for Cr in the corundum lattice is verified by fitting the Ti K-edge extended x-ray absorption fine structure (EXAFS) data. Room temperature electrical transport measurements confirm the highly resistive nature of Ti-doped Cr2O3, despite the presence of aliovalent Ti4+. For comparison, the resistivity of very pure, undoped Cr2O3 was measured to be four orders of magnitude higher than for Ti-doped Cr2O3. Analysis of the XPS and EXAFS data reveal the presence of Cr vacancies at intermediate and high Ti concentrations. This conclusion is corroborated by the results of density functional modeling. At low Ti concentrations, a strong increase of the XPS Ti 2p core level peak width is observed as the Ti concentration decreases. In this limit, the formation of Cr vacancies becomes less favorable due to the increased distance between Ti dopants, and compensation by O interstitials contributes to broadening of the Ti 2p XPS peak. The differences in electronic structure which render Ti4+-doped Cr2O3 resistive due to the formation of compensating defects, but Ti4+-doped Fe2O3 conductive, are discussed. The defect compensation model developed here provides insight into previous, conflicting reports of n-type versus p-type conductivity in Ti-doped Cr2O3 at high temperature, and will inform future studies to exploit the wide variety of electronic and magnetic properties of corundum structure oxides.
C1 [Kaspar, Tiffany C.; Sushko, Peter V.; Chambers, Scott A.] Pacific Northwest Natl Lab, Phys & Computat Sci Directorate, POB 999, Richland, WA 99352 USA.
[Bowden, Mark E.] Pacific Northwest Natl Lab, Environm Mol Sci Lab, POB 999, Richland, WA 99352 USA.
[Heald, Steve M.] Argonne Natl Lab, Adv Photon Source, 9700 S Cass Ave, Argonne, IL 60439 USA.
[Papadogianni, Alexandra; Tschammer, Carsten; Bierwagen, Oliver] Paul Drude Inst Festkorperelekt, Hausvogteipl 5-7, D-10117 Berlin, Germany.
RP Kaspar, TC (reprint author), Pacific Northwest Natl Lab, Phys & Computat Sci Directorate, POB 999, Richland, WA 99352 USA.
EM tiffany.kaspar@pnnl.gov
RI Sushko, Peter/F-5171-2013
OI Sushko, Peter/0000-0001-7338-4146
FU U.S. Department of Energy (DOE), Office of Science, Office of Basic
Energy Sciences (BES), Division of Materials Sciences and Engineering
[10122]; U.S. DOE's Office of Biological and Environmental Research; DOE
[DE-AC05-76RL01830]; DOE Office of Science [DE-AC02-06CH11357]
FX The authors are grateful to Vic Henrich for providing the synthetic
Ti2O3 single crystal. T.C.K., P.V.S., and S.A.C.
performed sample synthesis, characterization, data analysis, and
theoretical simulations with support from the U.S. Department of Energy
(DOE), Office of Science, Office of Basic Energy Sciences (BES),
Division of Materials Sciences and Engineering, under Award No. 10122.
A.P., C.T., and O.B. performed electrical transport measurements and
associated data analysis and acknowledge W. Seidel and B. Drescher for
processing. A portion of this work was performed using EMSL, a national
scientific user facility sponsored by the U.S. DOE's Office of
Biological and Environmental Research and located at the Pacific
Northwest National Laboratory (PNNL). PNNL is a multiprogram national
laboratory operated for DOE by Battelle under Contract No.
DE-AC05-76RL01830. XAS data were collected on an XSD beamline 20-BM of
the Advanced Photon Source, a U.S. Department of Energy (DOE) Office of
Science User Facility operated for the DOE Office of Science by Argonne
National Laboratory under Contract No. DE-AC02-06CH11357.
NR 51
TC 0
Z9 0
U1 11
U2 11
PU AMER PHYSICAL SOC
PI COLLEGE PK
PA ONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA
SN 2469-9950
EI 2469-9969
J9 PHYS REV B
JI Phys. Rev. B
PD OCT 7
PY 2016
VL 94
IS 15
AR 155409
DI 10.1103/PhysRevB.94.155409
PG 12
WC Physics, Condensed Matter
SC Physics
GA DY6MU
UT WOS:000385242200006
ER
PT J
AU Wang, YS
Feng, YJ
Cheng, JG
Wu, W
Luo, JL
Rosenbaum, TF
AF Wang, Yishu
Feng, Yejun
Cheng, J. -G.
Wu, W.
Luo, J. L.
Rosenbaum, T. F.
TI Spiral magnetic order and pressure-induced superconductivity in
transition metal compounds
SO NATURE COMMUNICATIONS
LA English
DT Article
ID QUANTUM-CRITICAL-POINT; X-RAY-SCATTERING; MNP; FLUCTUATIONS; CRAS
AB Magnetic and superconducting ground states can compete, cooperate and coexist. MnP provides a compelling and potentially generalizable example of a material where superconductivity and magnetism may be intertwined. Using a synchrotron-based non-resonant X-ray magnetic diffraction technique, we reveal a spiral spin order in MnP and trace its pressure evolution towards superconducting order via measurements in a diamond anvil cell. Judging from the magnetostriction, ordered moments vanish at the quantum phase transition as pressure increases the electron kinetic energy. Spins remain local in the disordered phase, and the promotion of superconductivity is likely to emerge from an enhanced coupling to residual spiral spin fluctuations and their concomitant suppression of phonon-mediated superconductivity. As the pitch of the spiral order varies across the 3d transition metal compounds in the MnP family, the magnetic ground state switches between antiferromagnet and ferromagnet, providing an additional tuning parameter in probing spin-fluctuation-induced superconductivity.
C1 [Wang, Yishu; Feng, Yejun; Rosenbaum, T. F.] CALTECH, Div Phys Math & Astron, Pasadena, CA 91125 USA.
[Feng, Yejun] Argonne Natl Lab, Adv Photon Source, Argonne, IL 60439 USA.
[Cheng, J. -G.; Wu, W.; Luo, J. L.] Chinese Acad Sci, Beijing Natl Lab Condensed Matter Phys, Beijing 100190, Peoples R China.
[Cheng, J. -G.; Wu, W.; Luo, J. L.] Chinese Acad Sci, Inst Phys, Beijing 100190, Peoples R China.
[Luo, J. L.] Collaborat Innovat Ctr Quantum Matter, Beijing 100190, Peoples R China.
RP Feng, YJ; Rosenbaum, TF (reprint author), CALTECH, Div Phys Math & Astron, Pasadena, CA 91125 USA.; Feng, YJ (reprint author), Argonne Natl Lab, Adv Photon Source, Argonne, IL 60439 USA.
EM yejun@anl.gov; tfr@caltech.edu
RI Feng, Yejun/A-5417-2009
OI Feng, Yejun/0000-0003-3667-056X
FU NSF [DMR-1420709]; U.S. Department of Energy Basic Energy Sciences
[DE-SC0014866]; U.S. Department of Energy Office of Science User
Facilities [DE-AC02-06CH11357]; MOST of China; NSF of China; Strategic
Priority Research Program of the Chinese Academy of Sciences
FX We thank P.B. Littlewood for helpful conversations. We are grateful to
B. Fisher for assisting with the magnetization measurements. Sample
preparation at the MRSEC facilities of the University of Chicago was
supported by NSF Grant No. DMR-1420709. The work at the California
Institute of Technology was supported by U.S. Department of Energy Basic
Energy Sciences Award DE-SC0014866. The use of the Advanced Photon
Source and the Center for Nanoscale Materials of Argonne National
Laboratory was supported by the U.S. Department of Energy Office of
Science User Facilities under contract No. DE-AC02-06CH11357. J.-G.C.
and J.L.L. were supported by the MOST and NSF of China, and the
Strategic Priority Research Program of the Chinese Academy of Sciences.
NR 45
TC 2
Z9 2
U1 10
U2 10
PU NATURE PUBLISHING GROUP
PI LONDON
PA MACMILLAN BUILDING, 4 CRINAN ST, LONDON N1 9XW, ENGLAND
SN 2041-1723
J9 NAT COMMUN
JI Nat. Commun.
PD OCT 6
PY 2016
VL 7
AR 13037
DI 10.1038/ncomms13037
PG 9
WC Multidisciplinary Sciences
SC Science & Technology - Other Topics
GA EH6LQ
UT WOS:000391885000001
PM 27708255
ER
PT J
AU Aaboud, M
Aad, G
Abbott, B
Abdallah, J
Abdinov, O
Abeloos, B
Aben, R
AbouZeid, OS
Abraham, NL
Abramowicz, H
Abreu, H
Abreu, R
Abulaiti, Y
Acharya, BS
Adamczyk, L
Adams, DL
Adelman, J
Adomeit, S
Adye, T
Affolder, AA
Agatonovic-Jovin, T
Agricola, J
Aguilar-Saavedra, JA
Ahlen, SP
Ahmadov, F
Aielli, G
Akerstedt, H
Aring;kesson, TPA
Akimov, AV
Alberghi, GL
Albert, J
Albrand, S
Verzini, MJA
Aleksa, M
Aleksandrov, IN
Alexa, C
Alexander, G
Alexopoulos, T
Alhroob, M
Ali, B
Aliev, M
Alimonti, G
Alison, J
Alkire, SP
Allbrooke, BMM
Allen, BW
Allport, PP
Aloisio, A
Alonso, A
Alonso, F
Alpigiani, C
Alstaty, M
Gonzalez, BA
Piqueras, DA
Alviggi, MG
Amadio, BT
Amako, K
Coutinho, YA
Amelung, C
Amidei, D
Dos Santos, SPA
Amorim, A
Amoroso, S
Amundsen, G
Anastopoulos, C
Ancu, LS
Andari, N
Andeen, T
Anders, CF
Anders, G
Anders, JK
Anderson, KJ
Andreazza, A
Andrei, V
Angelidakis, S
Angelozzi, I
Anger, P
Angerami, A
Anghinolfi, F
Anisenkov, AV
Anjos, N
Annovi, A
Antel, C
Antonelli, M
Antonov, A
Anulli, F
Aoki, M
Bella, LA
Arabidze, G
Arai, Y
Araque, JP
Arce, ATH
Arduh, FA
Arguin, JF
Argyropoulos, S
Arik, M
Armbruster, AJ
Armitage, LJ
Arnaez, O
Arnold, H
Arratia, M
Arslan, O
Artamonov, A
Artoni, G
Artz, S
Asai, S
Asbah, N
Ashkenazi, A
Aring;sman, B
Asquith, L
Assamagan, K
Astalos, R
Atkinson, M
Atlay, NB
Augsten, K
Avolio, G
Axen, B
Ayoub, MK
Azuelos, G
Baak, MA
Baas, AE
Baca, MJ
Bachacou, H
Bachas, K
Backes, M
Backhaus, M
Bagiacchi, P
Bagnaia, P
Bai, Y
Baines, JT
Baker, OK
Baldin, EM
Balek, P
Balestri, T
Balli, F
Balunas, WK
Banas, E
Banerjee, S
Bannoura, AAE
Barak, L
Barberio, EL
Barberis, D
Barbero, M
Barillari, T
Barisits, MS
Barklow, T
Barlow, N
Barnes, SL
Barnett, BM
Barnett, RM
Barnovska, Z
Baroncellia, A
Barone, G
Barr, AJ
Navarro, LB
Barreiro, F
da Costa, JBG
Bartoldus, R
Barton, AE
Bartos, P
Basalaev, A
Bassalat, A
Bates, RL
Batista, SJ
Batley, JR
Battaglia, M
Bauce, M
Bauer, F
Bawa, HS
Beacham, JB
Beattie, MD
Beau, T
Beauchemin, PH
Bechtle, P
Beck, HP
Becker, K
Becker, M
Beckingham, M
Becot, C
Beddall, AJ
Beddall, A
Bednyakov, VA
Bedognetti, M
Bee, CP
Beemster, LJ
Beermann, TA
Begel, M
Behr, JK
Belanger-Champagne, C
Bell, AS
Bella, G
Bellagamba, L
Bellerive, A
Bellomo, M
Belotskiy, K
Beltramello, O
Belyaev, NL
Benary, O
Benchekroun, D
Bender, M
Bendtz, K
Beneko, N
Benhammou, Y
Noccioli, EB
Benitez, J
Benjamin, DP
Bensinger, JR
Bentvelsen, S
Beresford, L
Beretta, M
Berge, D
Kuutmann, EB
Berger, N
Beringer, J
Berlendis, S
Bernard, NR
Bernius, C
Bernlochner, FU
Berry, T
Berta, P
Bertella, C
Bertoli, G
Bertolucci, F
Bertram, IA
Bertsche, C
Bertsche, D
Besjes, GJ
Bylund, OB
Bessner, M
Besson, N
Betancourt, C
Bethani, A
Bethke, S
Bevan, AJ
Bianchi, RM
Bianchini, L
Bianco, M
Biebel, O
Biedermann, D
Bielski, R
Biesuz, NV
Biglietti, M
De Mendizabal, JB
Billoud, TRV
Bilokon, H
Bindi, M
Binet, S
Bingul, A
Bini, C
Biondi, S
Bisanz, T
Bjergaard, DM
Black, CW
Black, JE
Black, KM
Blackburn, D
Blair, RE
Blanchard, JB
Blazek, T
Bloch, I
Blocker, C
Blum, W
Blumenschein, U
Blunier, S
Bobbink, GJ
Bobrovnikov, VS
Bocchetta, SS
Bocci, A
Bock, C
Boehler, M
Boerner, D
Bogaerts, JA
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CA ATLAS Collaboration
TI Search for bottom squark pair production in proton-proton collisions at
root s=13 TeV with the ATLAS detector
SO EUROPEAN PHYSICAL JOURNAL C
LA English
DT Article
ID PARTON DISTRIBUTIONS; HADRON COLLIDERS; PLUS PLUS; SUPERSYMMETRY;
PARTICLE; EXTENSION; DECAY; WEAK; LHC
AB The result of a search for pair production of the supersymmetric partner of the Standard Model bottom quark ((b) over tilde (1)) is reported. The search uses 3.2 fb(-1) of pp collisions at root s = 13 TeV collected by the ATLAS experiment at the Large Hadron Collider in 2015. Bottom squarks are searched for in events containing large missing transverse momentum and exactly two jets identified as originating from b-quarks. No excess above the expected Standard Model background yield is observed. Exclusion limits at 95 % confidence level on the mass of the bottom squark are derived in phenomenological supersymmetric R-parity-conserving models in which the (b) over tilde (1) is the lightest squark and is assumed to decay exclusively via (b) over tilde (1) -> b (chi) over tilde (0)(1), where (chi) over tilde (0)(1) is the lightest neutralino. The limits significantly extend previous results; bottom squark masses up to 800 (840) GeV are excluded for the. (chi) over tilde (0)(1) mass below 360 (100) GeV whilst differences in mass above 100 GeV between the (b) over tilde (1) and the (chi) over tilde (0)(1) are excluded up to a (b) over tilde (1) mass of 500 GeV.
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[Alonso, A.; Besjes, G. J.; Dam, M.; Galster, G.; Hansen, J. B.; Hansen, J. D.; Hansen, P. H.; Loevschall-Jensen, A. E.; Monk, J.; Mortensen, S. S.; Pedersen, L. E.; Petersen, T. C.; Pingel, A.; Wiglesworth, C.; Xella, S.] Univ Copenhagen, Niels Bohr Inst, Copenhagen, Denmark.
[Cairo, V. M.; Callea, G.; Capua, M.; Crosetti, G.; Del Gaudio, M.; La Rotonda, L.; Mastroberardino, A.; Palazzo, S.; Policicchio, A.; Salvatore, D.; Scarfone, V.; Schioppa, M.; Susinno, G.; Tassi, E.] Ist Nazl Fis Nucl, Grp Collegato Cosenza, Lab Nazl Frascati, Frascati, Italy.
[Cairo, V. M.; Callea, G.; Capua, M.; Crosetti, G.; Del Gaudio, M.; La Rotonda, L.; Mastroberardino, A.; Palazzo, S.; Policicchio, A.; Salvatore, D.; Scarfone, V.; Schioppa, M.; Susinno, G.; Tassi, E.] Univ Calabria, Dipartimento Fis, Arcavacata Di Rende, Italy.
[Adamczyk, L.; Bold, T.; Dabrowski, W.; Gach, G. P.; Grabowska-Bold, I.; Kisielewska, D.; Koperny, S.; Kowalski, T. Z.; Mindur, B.; Przybycien, M.; Schaile, D.; Zemla, A.] AGH Univ Sci & Technol, Fac Phys & Appl Comp Sci, Krakow, Poland.
[Palka, M.; Richter-Was, E.] Jagiellonian Univ, Marian Smoluchowski Inst Phys, Krakow, Poland.
[Banas, E.; De Renstrom, P. A. Bruckman; Burka, K.; Chwastowski, J. J.; Derendarz, D.; Godlewski, J.; Gornicki, E.; Hajduk, Z.; Iwanski, W.; Kaczmarska, A.; Knapik, J.; Korcyl, K.; Kowalewska, A. B.; Malecki, Pa.; Olszewski, A.; Olszowska, J.; Schaile, D.; Stanecka, E.; Staszewski, R.; Trzebinski, M.; Trzupek, A.; Wolter, M. W.; Wosiek, B. K.; Wozniak, K. W.; Zabinski, B.] Polish Acad Sci, Inst Nucl Phys, Krakow, Poland.
[Cao, T.; Firan, A.; Gupta, R.; Hetherly, J. W.; Kama, S.; Kehoe, R.; Sekula, S. J.; Stroynowski, R.; Turvey, A. J.; Varol, T.; Wang, H.; Ye, J.; Zhao, X.; Zhou, L.] So Methodist Univ, Dept Phys, Dallas, TX 75275 USA.
[Izen, J. M.; Leyton, M.; Meirose, B.; Namasivayam, H.; Reeves, K.] Univ Texas Dallas, Dept Phys, Richardson, TX 75083 USA.
[Behr, J. K.; Bertsche, C.; Bloch, I.; Britzger, D.; Deterre, C.; Dutta, B.; Eckardt, C.; Bravo, A. Gascon; Gasnikova, K.; Glazov, A.; Gregor, I. M.; Howarth, J.; Katzy, J.; Keller, J. S.; Lobodzinska, E.; Lohwasser, K.; Madsen, A.; Moenig, K.; O'Rourke, A. A.; Pirumov, H.; Poley, A.; Robinson, J. E. M.; Schaile, D.; South, D.; Trofymov, A.; Wang, J.] DESY, Zeuthen, Germany.
[Burmeister, I.; Cinca, D.; Dette, K.; Erdmann, J.; Esch, H.; Goessling, C.; Homann, M.; Klingenberg, R.; Kroeninger, K.] Tech Univ Dortmund, Lehrstuhl Expt Phys 4, Dortmund, Germany.
[Anger, P.; Duschinger, D.; Friedrich, F.; Grohs, J. P.; Gutschow, C.; Hauswald, L.; Kobel, M.; Mader, W. F.; Novgorodova, O.; Siegert, F.; Socher, F.; Straessner, A.; Vest, A.; Wahrmund, S.] Tech Univ Dresden, Inst Kern & Teilchenphys, Dresden, Germany.
[Arce, A. T. H.; Benjamin, D. P.; Bjergaard, D. M.; Bocci, A.; Cerio, B. C.; Goshaw, A. T.; Kajomovitz, E.; Kotwal, A.; Kruse, M. C.; Li, L.; Li, S.; Liu, M.; Oh, S. H.; Zhou, C.] Duke Univ, Dept Phys, Durham, NC 27706 USA.
[Bristow, T. M.; Clark, P. J.; Dias, F. A.; Edwards, N. C.; Gao, Y.; Walls, F. M. Garay; Glaysher, P. C. F.; Harrington, R. D.; Leonidopoulos, C.; Martin, V. J.; Mijovic, L.; Mills, C.; Pino, S. A. Olivares; Washbrook, A.; Wynne, B. M.] Univ Edinburgh, SUPA Sch Phys & Astron, Edinburgh, Midlothian, Scotland.
[Antonelli, M.; Beretta, M.; Bilokon, H.; Chiarella, V.; Curatolo, M.; Esposito, B.; Gatti, C.; Laurelli, P.; Maccarrone, G.; Mancini, G.; Sansoni, A.; Testa, M.; Vilucchi, E.] Ist Nazl Fis Nucl, Lab Nazl Frascati, Frascati, Italy.
[Arnold, H.; Betancourt, C.; Boehler, M.; Bruneliere, R.; Buehrer, F.; Burgard, C. D.; Buescher, D.; Cardillo, F.; Coniavitis, E.; Consorti, V.; Dang, N. P.; Dao, V.; Di Simone, A.; Glatzer, J.; Gonella, G.; Herten, G.; Hirose, M.; Jakobs, K.; Javurek, T.; Jenni, P.; Kiss, F.; Koeneke, K.; Kopp, A. K.; Kuehn, S.; Landgraf, U.; Luedtke, C.; Nagel, M.; Pagacova, M.; Parzefall, U.; Ronzani, M.; Rosbach, K.; Ruehr, F.; Rurikova, Z.; Sammel, D.; Schillo, C.; Schnoor, U.; Schumacher, M.; Sommer, P.; Sundermann, J. E.; Ta, D.; Temming, K. K.; Tsiskaridze, V.; Weiser, C.; Werner, M.; Zhang, L.; Zimmermann, S.] Albert Ludwigs Univ, Fak Math & Phys, Freiburg, Germany.
[Ancu, L. S.; De Mendizabal, J. Bilbao; Calace, N.; Chatterjee, A.; Clark, A.; Coccaro, A.; Delitzsch, C. M.; Della Volpe, D.; Ferrere, D.; Gadomski, S.; Golling, T.; Gonzalez-Sevilla, S.; Gramling, J.; Guescini, F.; Iacobucci, G.; Katre, A.; Khoo, T. J.; Lanfermann, M. C.; Lionti, A. E.; March, L.; Mermod, P.; Nackenhorst, O.; Paolozzi, L.; Ristie, B.; Schramm, S.; Sfyrla, A.; Wu, X.] Univ Geneva, Sect Phys, Geneva, Switzerland.
[Barberis, D.; Darbo, G.; Favareto, A.; Parodi, A. Ferretto; Gagliardi, G.; Gaudiello, A.; Gemme, C.; Guido, E.; Miglioranzi, S.; Morettini, P.; Osculati, B.; Parodi, F.; Passaggio, S.; Rossi, L. P.; Sannino, M.; Schiavi, C.] Ist Nazl Fis Nucl, Sez Genova, Genoa, Italy.
[Barberis, D.; Favareto, A.; Parodi, A. Ferretto; Gagliardi, G.; Gaudiello, A.; Guido, E.; Miglioranzi, S.; Osculati, B.; Parodi, F.; Sannino, M.; Schiavi, C.] Univ Genoa, Dipartimento Fis, Genoa, Italy.
[Jejelava, J.; Tskhadadze, E. G.] Iv Javakhishvili Tbilisi State Univ, E Andronikashvili Inst Phys, Tbilisi, Rep of Georgia.
[Djobava, T.; Durglishvili, A.; Khubua, J.; Mosidze, M.] Tbilisi State Univ, Inst High Energy Phys, Tbilisi, Rep of Georgia.
[Dueren, M.; Heinz, C.; Kreutzfeldt, K.; Stenzel, H.] Justus Liebig Univ Giessen, Phys Inst 2, Giessen, Germany.
[Bates, R. L.; Boutle, S. K.; Madden, W. D. Breaden; Britton, D.; Buckley, A. G.; Bussey, P.; Buttar, C. M.; Buzatu, A.; Crawley, S. J.; D'Auria, S.; Doyle, A. T.; Ferrando, J.; Gul, U.; Knue, A.; Mullen, P.; O'Shea, V.; Owen, M.; Pollard, C. S.; Qin, G.; Quilty, D.; Ravenscroft, T.; Robson, A.; Denis, R. D. St.; Stewart, G. A.; Thompson, A. S.] Univ Glasgow, SUPA Sch Phys & Astron, Glasgow, Lanark, Scotland.
[Agricola, J.; Bindi, M.; Bisanz, T.; Blumenschein, U.; Brandt, G.; De Maria, A.; Drechsler, E.; Graber, L.; Grosse-Knetter, J.; Janus, M.; Kareem, M. J.; Kawamura, G.; Lai, S.; Lemmer, B.; Magradze, E.; Mantoani, M.; Mchedlidze, G.; Llacer, M. Moreno; Musheghyan, H.; Quadt, A.; Rieger, J.; Rosien, N. -A.; Rzehorz, G. F.; Shabalina, E.; Stolte, P.; Veatch, J.; Weingarten, J.; Zinonos, Z.] Georg August Univ, Phys Inst 2, Gottingen, Germany.
[Albrand, S.; Berlendis, S.; Bethani, A.; Camincher, C.; Collot, J.; Crepe-Renaudin, S.; Delsart, P. A.; Gabaldon, C.; Genest, M. H.; Gradin, P. O. J.; Hostachy, J. -Y.; Ledroit-Guillon, F.; Lleres, A.; Lucotte, A.; Malek, F.; Petit, E.; Stark, J.; Trocme, B.; Wu, M.] Univ Grenoble Alpes, CNRS IN2P3, Lab Phys Subatom & Cosmol, Grenoble, France.
[Chan, S. K.; Clark, B. L.; Franklin, M.; Giromini, P.; Huth, J.; Ippolito, V.; Lazovich, T.; Mateos, D. Lopez; Morii, M.; Rogan, C. S.; Skottowe, H. P.; Sun, S.; Tolley, E.; Tong, B.; Tuna, A. N.; Yen, A. L.; Zambito, S.] Harvard Univ, Lab Particle Phys & Cosmol, Cambridge, MA 02138 USA.
[Andrei, V.; Antel, C.; Baas, A. E.; Brandt, O.; Djuvsland, J. I.; Dunford, M.; Geisler, M. P.; Hanke, P.; Jongmanns, J.; Kluge, E. -E.; Lang, V. S.; Meier, K.; Zu Theenhausen, H. Meyer; Villar, D. I. Narrias; Sahinsoy, M.; Schultz-Coulon, H. -C.; Stamen, R.; Starovoitov, P.; Suchek, S.; Wessels, M.] Heidelberg Univ, Kirchhoff Inst Phys, Heidelberg, Germany.
[Anders, C. F.; de Lima, D. E. Ferreira; Giulini, M.; Kolb, M.; Lisovyi, M.; Schaetzel, S.; Schoening, A.; Sosa, D.] Heidelberg Univ, Phys Inst, Heidelberg, Germany.
[Kretzc, M.; Kugel, A.] Heidelberg Univ, ZITI Inst Tech Informat, Mannheim, Germany.
[Nagasaka, Y.] Hiroshima Inst Technol, Fac Appl Informat Sci, Hiroshima, Japan.
[Bortolotto, V.; Chan, Y. L.; Castillo, L. R. Flores; Lu, H.; Salvucci, A.; Tsui, K. M.] Chinese Univ Hong Kong, Dept Phys, Shatin, Hong Kong, Peoples R China.
[Bortolotto, V.; Orlando, N.; Tu, Y.] Univ Hong Kong, Dept Phys, Pok Fu Lam, Hong Kong, Peoples R China.
[Bortolotto, V.; Prokofiev, K.] Hong Kong Univ Sci & Technol, Dept Phys, Clear Water Bay, Kowloon, Hong Kong, Peoples R China.
[Choi, K.; Dattagupta, A.; Evans, H.; Gagnon, P.; Kopeliansky, R.; Lammers, S.; Martinez, N. Lorenzo; Luehring, F.; Ogren, H.; Penwell, J.; Weinert, B.; Zieminska, D.] Indiana Univ, Dept Phys, Bloomington, IN 47405 USA.
[Guenther, J.; Jansky, R.; Kneringer, E.; Lukas, W.; Milic, A.; Usanova, A.] Leopold Franzens Univ, Inst Astro & Teilchenphys, Innsbruck, Austria.
[Abdallah, J.; Argyropoulos, S.; Benitez, J.; Mallik, U.] Univ Iowa, Iowa City, IA USA.
[Chen, C.; Cochran, J.; Jiang, H.; Krumnack, N.; Pluth, D.; Prell, S.; Werner, M. D.; Yu, J.] Iowa State Univ, Dept Phys & Astron, Ames, IA USA.
[Ahmadov, F.; Aleksandrov, I. N.; Bednyakov, V. A.; Boyko, I. R.; Budagov, I. A.; Chelkov, G. A.; Cheplakov, A.; Chizhov, M. V.; Dedovich, D. V.; Demichev, M.; Gongadze, A.; Gostkin, M. I.; Huseynov, N.; Javadov, N.; Karpov, S. N.; Karpova, Z. M.; Khramov, E.; Kruchonak, U.; Kukhtin, V.; Ladygin, E.; Lyubushkin, V.; Minashvili, I. A.; Mineev, M.; Peshekhonov, V. D.; Plotnikova, E.; Potrap, I. N.; Pozdnyakov, V.; Rusakovich, N. A.; Sadykov, R.; Sapronov, A.; Shiyakova, M.; Soloshenko, A.; Turchikhin, S.; Vinogradov, V. B.; Yeletskikh, I.; Zhemchugov, A.; Zimine, I.] JINR Dubna, Joint Inst Nucl Res, Dubna, Russia.
[Amako, K.; Aoki, M.; Arai, Y.; Hanagaki, K.; Ikegami, Y.; Ikeno, M.; Iwasaki, H.; Kanzaki, J.; Kondo, T.; Kono, T.; Makida, Y.; Nagai, R.; Nagano, K.; Nakamura, K.; Nozaki, M.; Odaka, S.; Okuyama, T.; Sasaki, O.; Schaile, D.; Suzuki, S.; Takubo, Y.; Tanaka, S.; Terada, S.; Tokushuku, K.; Tsuno, S.; Unno, Y.; Yamamoto, A.; Yasu, Y.] KEK, High Energy Accelerator Res Org, Tsukuba, Ibaraki, Japan.
[Chen, Y.; Hasegawa, M.; Kido, S.; Kurashige, H.; Maeda, J.; Ochi, A.; Shimizu, S.; Yamazaki, Y.; Yuan, L.] Kobe Univ, Grad Sch Sci, Kobe, Hyogo, Japan.
[Kunigo, T.; Monden, R.; Sumida, T.; Tashiro, T.] Kyoto Univ, Fac Sci, Kyoto, Japan.
[Takashima, R.] Kyoto Univ, Kyoto, Japan.
[Kawagoe, K.; Laforge, B.; Oda, S.; Otono, H.; Tojo, J.] Kyushu Univ, Dept Phys, Fukuoka, Japan.
[Verzini, M. J. Alconada; Alonso, F.; Arduh, F. A.; Dova, M. T.; Ji, H.; Monticelli, F.; Wahlberg, H.] Univ Nacl La Plata, Inst Fis La Plata, La Plata, Buenos Aires, Argentina.
[Verzini, M. J. Alconada; Alonso, F.; Arduh, F. A.; Dova, M. T.; Ji, H.; Monticelli, F.; Wahlberg, H.] Consejo Nacl Invest Cient & Tecn, La Plata, Buenos Aires, Argentina.
[Barton, A. E.; Beattie, M. D.; Bertram, I. A.; Borissov, G.; Bouhova-Thacker, E. V.; Cheatham, S.; Dearnaley, W. J.; Fox, H.; Grimm, K.; Henderson, R. C. W.; Hughes, G.; Jones, R. W. L.; Kartvelishvili, V.; Long, R. E.; Love, P. A.; Muenstermann, D.; Parker, A. J.; Skinner, M. B.; Smizanska, M.; Walder, J.; Wharton, A. M.] Univ Lancaster, Dept Phys, Lancaster, England.
[Aliev, M.; Bachas, K.; Chiodini, G.; Gorini, E.; Longo, L.; Primavera, M.; Reale, M.; Spagnolo, S.; Ventura, A.] Ist Nazl Fis Nucl, Sez Lecce, Lecce, Italy.
[Aliev, M.; Bachas, K.; Gorini, E.; Longo, L.; Reale, M.; Spagnolo, S.; Ventura, A.] Univ Salento, Dipartimento Matemat & Fis, Lecce, Italy.
[Affolder, A. A.; Anders, J. K.; Burdin, S.; D'Onofrio, M.; Dervan, P.; Gwilliam, C. B.; Hayward, H. S.; Jones, T. J.; King, B. T.; Klein, M.; Klein, U.; Kretzschmar, J.; Laycock, P.; Lehan, A.; Maxfield, S. J.; Mehta, A.; Readioff, N. P.; Vossebeld, J. H.] Univ Liverpool, Oliver Lodge Lab, Liverpool, Merseyside, England.
[Cindro, V.; Filipcic, A.; Gorisek, A.; Kanjir, L.; Kersevan, B. P.; Kramberger, G.; Macek, B.; Mandic, I.; Mikuz, M.; Muskinja, M.; Sfiligoj, T.; Sokhrannyi, G.] Jozef Stefan Inst, Dept Phys, Ljubljana, Slovenia.
[Cindro, V.; Filipcic, A.; Gorisek, A.; Kanjir, L.; Kersevan, B. P.; Kramberger, G.; Macek, B.; Mandic, I.; Mikuz, M.; Muskinja, M.; Sfiligoj, T.; Sokhrannyi, G.] Univ Ljubljana, Ljubljana, Slovenia.
[Armitage, L. J.; Bevan, A. J.; Bona, M.; Hays, J. M.; Hickling, R.; Landon, M. P. J.; Lewis, D.; Lloyd, S. L.; Morris, J. D.; Nooney, T.; Piccaro, E.; Rizvi, E.; Sandbach, R. L.] Queen Mary Univ London, Sch Phys & Astron, London, England.
[Berry, T.; Boisvert, V.; Brooks, T.; Connelly, I. A.; Cowan, G.; Giannelli, M. Faucci; George, S.; Gibson, S. M.; Kempster, J. J.; Kilby, C. R.; Vazquez, J. G. Panduro; Pastore, Fr.; Savage, G.; Sowden, B. C.; Spano, F.; Teixeira-Dias, P.; Thomas-Wilsker, J.] Royal Holloway Univ London, Dept Phys, Surrey, England.
[Bell, A. S.; Butterworth, J. M.; Campanelli, M.; Christodoulou, V.; Cooper, B. D.; Davison, P.; Falla, R. J.; Freeborn, D.; Gregersen, K.; Grout, Z. J.; Ortiz, N. G. Gutierrez; Hesketh, G. G.; Jansen, E.; Jiggins, S.; Konstantinidis, N.; Korn, A.; Kucuk, H.; Leney, K. J. C.; Martyniuk, A. C.; McClymont, L. I.; Mcfayden, J. A.; Nurse, E.; Richter, S.; Scanlon, T.; Sherwood, P.; Simmons, B.; Wardrope, D. R.; Waugh, B. M.] UCL, Dept Phys & Astron, London, England.
[Greenwood, Z. D.; Grossi, G. C.; Jana, D. K.; Sawyer, L.] Louisiana Tech Univ, Ruston, LA 71270 USA.
[Beau, T.; Bomben, M.; Calderini, G.; Crescioli, F.; De Groot, N.; Demilly, A.; Derue, F.; Francavilla, P.; Krasny, M. W.; Lacour, D.; Laplace, S.; LeDortz, O.; Lefebvre, G.; Solis, A. Lopez; Luzi, P. M.; Malaescu, B.; Marchiori, G.; Nikolic-Audit, I.; Ocariz, J.; Pandini, C. E.; Pires, S.; Ridel, M.; Roos, L.; Schaile, D.; Schamberger, R. D.; Trincaz-Duvoid, S.; Varouchas, D.; Yap, Y. C.] UPMC, Lab Phys Nucl & Hautes Energies, Paris, France.
[Beau, T.; Bomben, M.; Calderini, G.; Crescioli, F.; De Groot, N.; Demilly, A.; Derue, F.; Francavilla, P.; Krasny, M. W.; Lacour, D.; Laplace, S.; LeDortz, O.; Lefebvre, G.; Solis, A. Lopez; Luzi, P. M.; Malaescu, B.; Marchiori, G.; Nikolic-Audit, I.; Ocariz, J.; Pandini, C. E.; Pires, S.; Ridel, M.; Roos, L.; Trincaz-Duvoid, S.; Varouchas, D.; Yap, Y. C.] Univ Paris Diderot, Paris, France.
[Beau, T.; Bomben, M.; Calderini, G.; Crescioli, F.; De Groot, N.; Demilly, A.; Derue, F.; Francavilla, P.; Krasny, M. W.; Lacour, D.; Laplace, S.; LeDortz, O.; Lefebvre, G.; Solis, A. Lopez; Luzi, P. M.; Malaescu, B.; Marchiori, G.; Nikolic-Audit, I.; Ocariz, J.; Pandini, C. E.; Pires, S.; Ridel, M.; Roos, L.; Trincaz-Duvoid, S.; Varouchas, D.; Yap, Y. C.] CNRS IN2P3, Paris, France.
[Akesson, T. P. A.; Bocchetta, S. S.; Bryngemark, L.; Doglioni, C.; Floderus, A.; Hedberg, V.; Jarlskog, G.; Lytken, E.; Mjornmark, J. U.; Smirnova, O.; Viazlo, O.] Lund Univ, Fys Inst, Lund, Sweden.
[Barreiro, F.; Lopez, S. Calvente; Cueto, A.; De Lorenzi, F.; Del Peso, J.; Glasman, C.; Terron, J.] Univ Autonoma Madrid, Dept Fis Teor C 15, Madrid, Spain.
[Artz, S.; Becker, M.; Bertella, C.; Blum, W.; Buescher, V.; Caputo, R.; Cuth, J.; Dudder, A. Chr.; Endner, O. C.; Ertel, E.; Fiedler, F.; Torregrosa, E. Fullana; Geisen, M.; Groh, S.; Heck, T.; Jakobi, K. B.; Kaluza, A.; Karnevskiy, M.; Kleinknecht, K.; Koepke, L.; Lin, T. H.; Masetti, L.; Mattmann, J.; Meyer, C.; Moritz, S.; Pleskot, V.; Rave, S.; Sander, H. G.; Schaeffer, J.; Schaefer, U.; Schaile, D.; Schmitt, C.; Schmitz, S.; Schott, M.; Schuh, N.; Schulte, A.; Simioni, E.; Simon, M.; Tapprogge, S.; Urrejola, P.; Webb, S.; Yildirim, E.; Zimmermann, C.; Zinser, M.] Johannes Gutenberg Univ Mainz, Inst Phys, Mainz, Germany.
[Barnes, S. L.; Bielski, R.; Cox, B. E.; Da Via, C.; Dann, N. S.; Forcolin, G. T.; Forti, A.; Ponce, J. M. Iturbe; Li, X.; Loebinger, F. K.; Marsden, S. P.; Masik, J.; Sanchez, F. J. Munoz; Neep, T. J.; Oh, A.; Ospanov, R.; Pater, J. R.; Peters, R. F. Y.; Pilkington, A. D.; Pin, A. W. J.; Price, D.; Qin, Y.; Queitsch-Maitland, M.; Raine, J. A.; Schaile, D.; Schweiger, H.; Shaw, S. M.; Tomlinson, L.; Watts, S.; Wilk, F.; Woudstra, M. J.; Wyatt, T. R.] Univ Manchester, Sch Phys & Astron, Manchester, Lancs, England.
[Aad, G.; Alstaty, M.; Barbero, M.; Calandri, A.; Calvet, T. P.; Coadou, Y.; Diaconu, C.; Diglio, S.; Djama, F.; Ellajosyula, V.; Feligioni, L.; Gao, J.; Hadef, A.; Hallewell, G. D.; Hubaut, F.; Kahn, S. J.; Knoops, E. B. F. G.; LeGuirriec, E.; Liu, J.; Liu, K.; Madaffari, D.; Monnier, E.; Muanza, S.; Nagy, E.; Pralavorio, P.; Rodina, Y.; Rozanov, A.; Schaile, D.; Talby, M.; Theveneaux-Pelzer, T.; Torres, R. E. Ticse; Tisserant, S.; Toth, J.; Touchard, F.; Vacavant, L.; Wang, C.] Aix Marseille Univ, CPPM, Marseille, France.
[Aad, G.; Aloisio, A.; Alstaty, M.; Barbero, M.; Calandri, A.; Calvet, T. P.; Coadou, Y.; Diaconu, C.; Diglio, S.; Djama, F.; Ellajosyula, V.; Feligioni, L.; Gao, J.; Hadef, A.; Hallewell, G. D.; Hubaut, F.; Kahn, S. J.; Knoops, E. B. F. G.; LeGuirriec, E.; Liu, J.; Liu, K.; Madaffari, D.; Monnier, E.; Muanza, S.; Nagy, E.; Pralavorio, P.; Rodina, Y.; Rozanov, A.; Schaile, D.; Schamberger, R. D.; Talby, M.; Theveneaux-Pelzer, T.; Torres, R. E. Ticse; Tisserant, S.; Toth, J.; Touchard, F.; Vacavant, L.; Wang, C.] CNRS IN2P3, Marseille, France.
[Bellomo, M.; Bernard, N. R.; Brau, B.; Dallapiccola, C.; Daya-Ishmukhametova, R. K.; Moyse, E. J. W.; Pais, P.; Pettersson, N. E.; Picazio, A.; Schaile, D.; Willocq, S.] Univ Massachusetts, Dept Phys, Amherst, MA 01003 USA.
[Belanger-Champagne, C.; Chuinard, A. J.; Corriveau, F.; Keyes, R. A.; Lefebvre, B.; Mantifel, R.; Prince, S.; Robertson, S. H.; Robichaud-Veronneau, A.; Schaile, D.; Stockton, M. C.; Stoebe, M.; Vachon, B.; Schroeder, T. Vazquez; Wang, K.; Warburton, A.] McGill Univ, Dept Phys, Montreal, PQ, Canada.
[Barberio, E. L.; Dawe, E.; Goldfarb, S.; Jennens, D.; Kubota, T.; Le, B.; McDonald, E. F.; Milesi, M.; Nuti, F.; Rados, P.; Scutti, F.; Spiller, L. A.; Tan, K. G.; Taylor, G. N.; Taylor, P. T. E.; Ungaro, F. C.; Urquijo, P.; Volpi, M.; Zanzi, D.] Univ Melbourne, Sch Phys, Melbourne, Vic, Australia.
[Amidei, D.; Chelstowska, M. A.; Cheng, H. C.; Dai, T.; Diehl, E. B.; Edgar, R. C.; Feng, H.; Ferretti, C.; Fleischmann, P.; Guan, L.; Levin, D.; Liu, H.; Lu, N.; Marley, D. E.; Mc Kee, S. P.; McCarn, A.; Neal, H. A.; Qian, J.; Schwarz, T. A.; Searcy, J.; Sekhon, K.; Wu, Y.; Yu, J. M.; Zhang, D.; Zhou, B.; Zhu, J.] Univ Michigan, Dept Phys, Ann Arbor, MI 48109 USA.
[Arabidze, G.; Brock, R.; Chegwidden, A.; Fisher, W. C.; Halladjian, G.; Hauser, R.; Hayden, D.; Huston, J.; Mondragon, M. C.; Plucinski, P.; Pope, B. G.; Schoenrock, B. D.; Schwienhorst, R.; Willis, C.] Michigan State Univ, Dept Phys & Astron, E Lansing, MI 48824 USA.
[Alimonti, G.; Andreazza, A.; Camplani, A.; Carminati, L.; Cavalli, D.; Citterio, M.; Costa, G.; Fanti, M.; Giugni, D.; Lari, T.; Lazzaroni, M.; Mandelli, L.; Manzoni, S.; Mazza, S. M.; Meroni, C.; Monzani, S.; Perini, L.; Ragusa, F.; Ratti, M. G.; Resconi, S.; Shojaii, S.; Stabile, A.; Tartarelli, G. F.; Troncon, C.; Turra, R.; Perez, M. Villaplana] Ist Nazl Fis Nucl, Sez Milano, Milan, Italy.
[Andreazza, A.; Camplani, A.; Carminati, L.; Fanti, M.; Lazzaroni, M.; Manzoni, S.; Mazza, S. M.; Monzani, S.; Perini, L.; Ragusa, F.; Ratti, M. G.; Shojaii, S.; Turra, R.; Perez, M. Villaplana] Univ Milan, Dipartimento Fis, Milan, Italy.
[Harkusha, S.; Kulchitsky, Y.; Kurochkin, Y. A.; Tsiareshka, P. V.] Natl Acad Sci Belarus, BI Stepanov Inst Phys, Minsk, Byelarus.
[Hrynevich, A.] Natl Sci & Educ Ctr Particle & High Energy Phys, Minsk, Byelarus.
[Arguin, J. -F.; Azuelos, G.; Billoud, T. R. V.; Dallaire, F.; Ducu, O. A.; Gagnon, L. G.; Gauthier, L.; Leroy, C.; Mochizuki, K.; Manh, T. Nguyen; Rezvani, R.; Saadi, D. Shoaleh] Univ Montreal, Grp Particle Phys, Montreal, PQ, Canada.
[Akimov, A. V.; Gavrilenko, I. L.; Komar, A. A.; Mashinistov, R.; Mouraviev, S. V.; Nechaeva, P. Yu.; Shmeleva, A.; Snesarev, A. A.; Sulin, V. V.; Tikhomirov, V. O.; Zhukov, K.] Russian Acad Sci, PN Lebedev Phys Inst, Moscow, Russia.
[Artamonov, A.; Gorbounov, P. A.; Khovanskiy, V.; Shatalov, P. B.; Tsukerman, I. I.] Inst Theoret & Expt Phys ITEP, Moscow, Russia.
[Antonov, A.; Belotskiy, K.; Belyaev, N. L.; Brennan, A. J.; Bulekov, O.; Kantserov, V. A.; Krasnopevtsev, D.; Romaniouk, A.; Shulga, E.; Smirnov, S. Yu.; Smirnov, Y.; Soldatov, E. Yu.; Timoshenko, S.; Vorobev, K.] Natl Res Nucl Univ MEPhI, Moscow, Russia.
[Gladilin, L. K.; Kramarenko, V. A.; Maevskiy, A.; Sivoklokov, S. Yu.; Smirnova, L. N.] Moscow MV Lomonosov State Univ, DV Skobeltsyn Inst Nucl Phys, Moscow, Russia.
[Adomeit, S.; Bender, M.; Biebel, O.; Bock, C.; Calfayan, P.; Chow, B. K. B.; Duckeck, G.; Hartmann, N. M.; Heinrich, J. J.; Hertenberger, R.; Hoenig, F.; Legger, F.; Lorenz, J.; Loesel, P. J.; Maier, T.; Mann, A.; Mehlhase, S.; Meineck, C.; Mitrevski, J.; Mueller, R. S. P.; Rauscher, F.; Ruschke, A.; Schachtner, B. M.; Schaile, D.; Unverdorben, C.; Valderanis, C.; Walker, R.; Wittkowski, J.] Ludwig Maximilians Univ Munchen, Fak Phys, Munich, Germany.
[Giuliani, C.; Kiryunin, A. E.; La Rosa, A.; Macchiolo, A.; Maier, A. A.; Mueller, F.; Salihagic, D.; Spettel, F.; Wildauer, A.] Werner Heisenberg Inst, Max Planck Inst Phys, Munich, Germany.
[Fusayasu, T.; Shimojima, M.] Nagasaki Inst Appl Sci, Nagasaki, Japan.
[Horii, Y.; Kentaro, K.; Nakahama, Y.; Onogi, K.; Tomoto, M.; Wakabayashi, J.; Yamauchi, K.] Nagoya Univ, Grad Sch Sci, Nagoya, Aichi, Japan.
[Horii, Y.; Kentaro, K.; Nakahama, Y.; Onogi, K.; Tomoto, M.; Wakabayashi, J.; Yamauchi, K.] Nagoya Univ, Kobayashi Maskawa Inst, Nagoya, Aichi, Japan.
[Aloisio, A.; Alviggi, M. G.; Canale, V.; Cirotto, F.; Conventi, F.; de Asmundis, R.; Della Pietra, M.; Doria, A.; Izzo, V.; Merola, L.; Perrella, S.; Rossi, E.; Sanchez, A.; Sekhniaidze, G.] Ist Nazl Fis Nucl, Sez Napoli, Naples, Italy.
[Aloisio, A.; Alviggi, M. G.; Canale, V.; Cirotto, F.; Merola, L.; Perrella, S.; Rossi, E.; Sanchez, A.] Univ Napoli, Dipartimento Fis, Naples, Italy.
[Gorelov, I.; Hoeferkamp, M. R.; Mc Fadden, N. C.; Seidel, S. C.; Taylor, A. C.; Toms, K.] Univ New Mexico, Dept Phys & Astron, Albuquerque, NM 87131 USA.
[Caron, S.; Colasurdo, L.; Croft, V.; de Jong, P.; Filthaut, F.; Galea, C.; Konig, A. C.; Nektarijevic, S.; Strubig, A.] Radboud Univ Nijmegen Nikhef, Inst Math Astrophys & Particle Phys, Nijmegen, Netherlands.
[Aben, R.; Angelozzi, I.; Bedognetti, M.; Beemster, L. J.; Bentvelsen, S.; Berge, D.; Bobbink, G. J.; Bos, K.; Brenner, L.; Bruni, L. S.; Butti, P.; Castelijn, R.; Castelli, A.; Colijn, A. P.; De la Torre, H.; Deigaard, I.; Duda, D.; Ferrari, P.; Hartjes, F.; Hessey, N. P.; Igonkina, O.; Kluit, P.; Koffeman, E.; Mahlstedt, J.; Meyer, J.; Oussoren, K. P.; Sabato, G.; Salek, D.; Slawinska, M.; Talyshev, A. A.; Valencic, N.; Van Den Wollenberg, W.; Van Der Deijl, P. C.; van der Graaf, H.; van Vulpen, I.; Vankov, P.; Verkerke, W.; Vermeulen, J. C.; Vreeswijk, M.; Weits, H.; Williams, S.; Wolf, T. M. H.] Nikhef Natl Inst Subat Phys, Amsterdam, Netherlands.
[Aben, R.; Angelozzi, I.; Bedognetti, M.; Beemster, L. J.; Bentvelsen, S.; Berge, D.; Bobbink, G. J.; Bos, K.; Brenner, L.; Bruni, L. S.; Butti, P.; Castelijn, R.; Castelli, A.; Colijn, A. P.; De la Torre, H.; Deigaard, I.; Duda, D.; Ferrari, P.; Hartjes, F.; Hessey, N. P.; Igonkina, O.; Kluit, P.; Koffeman, E.; Mahlstedt, J.; Meyer, J.; Oussoren, K. P.; Sabato, G.; Salek, D.; Slawinska, M.; Talyshev, A. A.; Valencic, N.; Van Den Wollenberg, W.; Van Der Deijl, P. C.; van der Graaf, H.; van Vulpen, I.; Vankov, P.; Verkerke, W.; Vermeulen, J. C.; Vreeswijk, M.; Weits, H.; Williams, S.; Wolf, T. M. H.] Univ Amsterdam, Amsterdam, Netherlands.
[Adelman, J.; Brost, E.; Burghgrave, B.; Chakraborty, D.; Klimek, P.; Saha, P.] Univ Illinois, Dept Phys, De Kalb, IL USA.
[Anisenkov, A. V.; Baldin, E. M.; Bobrovnikov, V. S.; Bogdanchikov, A. G.; Buzykaev, A. R.; Kazanin, V. F.; Kharlamov, A. G.; Korol, A. A.; Maslennikov, A. L.; Maximov, D. A.; Peleganchuk, S. V.; Rezanova, O. L.; Soukharev, A. M.; Tikhonov, Yu. A.] SB RAS, Budker Inst Nucl Phys, Novosibirsk, Russia.
[Becot, C.; Bernius, C.; Cranmer, K.; Haas, A.; Heinrich, L.; Kaplan, B.; Karthik, K.; Konoplich, R.; Mincer, A. I.; Nemethy, P.; Neves, R. M.] NYU, Dept Phys, 4 Washington Pl, New York, NY 10003 USA.
[Beacham, J. B.; Che, S.; Gan, K. K.; Ishmukhametov, R.; Kagan, H.; Kass, R. D.; Looper, K. A.; Shrestha, S.; Tannenwald, B. B.] Ohio State Univ, Columbus, OH 43210 USA.
[Nakano, I.] Okayama Univ, Fac Sci, Okayama, Japan.
[Abbott, B.; Alhroob, M.; Bertsche, D.; De Benedetti, A.; Gutierrez, P.; Hasib, A.; Norberg, S.; Pearson, B.; Rifki, O.; Severini, H.; Skubic, P.; Strauss, M.] Univ Oklahoma, Homer L Dodge Dept Phys & Astron, Norman, OK 73019 USA.
[Cantero, J.; Haley, J.; Jamin, D. O.; Khanov, A.; Rizatdinova, F.; Sidorov, D.] Oklahoma State Univ, Dept Phys, Stillwater, OK 74078 USA.
[Chytka, L.; Hamal, P.; Hrabovsky, M.; Kvita, J.; Nozka, L.] Palacky Univ, RCPTM, Olomouc, Czech Republic.
[Abreu, R.; Allen, B. W.; Brau, J. E.; Hopkins, W. H.; Majewski, S.; Potter, C. T.; Radloff, P.; Sinev, N. B.; Strom, D. M.; Torrence, E.; Wanotayaroj, C.; Whalen, K.; Winklmeier, F.] Univ Oregon, Ctr High Energy Phys, Eugene, OR 97403 USA.
[Abeloos, B.; Ayoub, M. K.; Bassalat, A.; Binet, S.; Bourdarios, C.; De Regie, J. B. De Vivie; Delgove, D.; Duflot, L.; Escalier, M.; Fayard, L.; Fournier, D.; Gkougkousis, E. L.; Goudet, C. R.; Grivaz, J. -F.; Hariri, F.; Henrot-Versille, S.; Hrivnac, J.; Iconomidou-Fayard, L.; Kado, M.; Lounis, A.; Maiani, C.; Makovec, N.; Morange, N.; Nellist, C.; Petroff, P.; Poggioli, L.; Puzo, P.; Rousseau, D.; Rybkin, G.; Schaffer, A. C.; Schaile, D.; Serin, L.; Simion, S.; Tanaka, R.; Zerwas, D.; Zhang, Z.] Univ Paris Saclay, Univ Paris Sud, CNRS IN2P3, LAL, Orsay, France.
[Ishijima, N.; Nomachi, M.; Sugaya, Y.; Teoh, J. J.; Yamaguchi, Y.] Osaka Univ, Grad Sch Sci, Osaka, Japan.
[Bugge, M. K.; Cameron, D.; Catmore, J. R.; Feigl, S.; Franconi, L.; Garonne, V.; Gjelsten, B. K.; Gramstad, E.; Morisbak, V.; Nilsen, J. K.; Ould-Saada, F.; Pajchel, K.; Pedersen, M.; Raddum, S.; Read, A. L.; Rohne, O.; Sandaker, H.; Serfon, C.; Stapnes, S.; Strandlie, A.] Univ Oslo, Dept Phys, Oslo, Norway.
[Artoni, G.; Barr, A. J.; Becker, K.; Beresford, L.; Bortoletto, D.; Burr, J. T. P.; Cooper-Sarkar, A. M.; Ortuzar, M. Crispin; Fawcett, W. J.; Frost, J. A.; Gallas, E. J.; Giuli, F.; Gupta, S.; Gwenlan, C.; Hays, C. P.; Henderson, J.; Huffman, T. B.; Issever, C.; Kalderon, C. W.; Nagai, K.; Nickerson, R. B.; Norjoharuddeen, N.; Petrov, M.; Pickering, M. A.; Radescu, V.; Schaile, D.; Schamberger, R. D.; Tseng, J. C. -L.; Viehhauser, G. H. A.; Vigani, L.; Weidberg, A. R.; Zhong, J.] Univ Oxford, Dept Phys, Oxford, England.
[Dondero, P.; Farina, E. M.; Ferrari, R.; Fraternali, M.; Gaudio, G.; Introzzi, G.; Kourkoumeli-Charalampidi, A.; Lanza, A.; Livan, M.; Negri, A.; Polesello, G.; Rebuzzi, D. M.; Rimoldi, A.; Vercesi, V.] Ist Nazl Fis Nucl, Sez Pavia, Pavia, Italy.
[Dondero, P.; Farina, E. M.; Fraternali, M.; Introzzi, G.; Kourkoumeli-Charalampidi, A.; Livan, M.; Negri, A.; Rebuzzi, D. M.; Rimoldi, A.] Univ Pavia, Dipartimento Fis, Pavia, Italy.
[Balunas, W. K.; Brendlinger, K.; Di Clemente, W. K.; Fletcher, R. R. M.; Haney, B.; Heim, S.; Hines, E.; Jackson, B.; Kroll, J.; Lipeles, E.; Miguens, J. Machado; Meyer, C.; Mistry, K. P.; Reichert, J.; Schaefer, L.; Thomson, E.; Vanguri, R.; Williams, H. H.; Yoshihara, K.] Univ Penn, Dept Phys, Philadelphia, PA 19104 USA.
[Basalaev, A.; Ezhilov, A.; Fedin, O. L.; Gratchev, V.; Levchenko, M.; Maleev, V. P.; Naryshkin, I.; Ryabov, Y. F.; Schaile, D.; Schegelsky, V. A.; Seliverstov, D. M.; Solovyev, V.] BP Konstantinov Petersburg Nucl Phys Inst, Kurchatov Inst, Natl Res Ctr, St Petersburg, Russia.
[Annovi, A.; Bertolucci, F.; Biesuz, N. V.; Cavasinni, V.; Chiarelli, G.; Del Prete, T.; Dell'Orso, M.; Donati, S.; Giannetti, P.; Leone, S.; Roda, C.; Schaile, D.; Scuri, F.; Sotiropoulou, C. L.; Spalla, M.; Stanescu, C.; Volpi, G.] Ist Nazl Fis Nucl, Sez Pisa, Pisa, Italy.
[Annovi, A.; Bertolucci, F.; Biesuz, N. V.; Cavasinni, V.; Chiarelli, G.; Del Prete, T.; Dell'Orso, M.; Donati, S.; Giannetti, P.; Leone, S.; Roda, C.; Scuri, F.; Sotiropoulou, C. L.; Spalla, M.; Volpi, G.] Univ Pisa, Dipartimento Fis E Fermi, Pisa, Italy.
[Bianchi, R. M.; Boudreau, J.; Escobar, C.; Farina, C.; Hong, T. M.; Mueller, J.; Sapp, K.; Su, J.] Univ Pittsburgh, Dept Phys & Astron, Pittsburgh, PA 15260 USA.
[Aguilar-Saavedra, J. A.; Dos Santos, S. P. Amor; Amorim, A.; Araque, J. P.; Cantrill, R.; Carvalho, J.; Castro, N. F.; Muino, P. Conde; Da Cunha Sargedas De Sousa, M. J.; Fiolhais, M. C. N.; Galhardo, B.; Gomes, A.; Goncalo, R.; Jorge, P. M.; Lopes, L.; Maio, A.; Maneira, J.; Seabra, L. F. Oleiro; Onofre, A.; Pedro, R.; Santos, H.; Saraiva, J. G.; Silva, J.; Delgado, A. Tavares; Veloso, F.; Wolters, H.] LIP, Lab Instrumentacao & Fis Expt Particulas, Lisbon, Portugal.
[Amorim, A.; Muino, P. Conde; Da Cunha Sargedas De Sousa, M. J.; Gomes, A.; Jorge, P. M.; Miguens, J. Machado; Maio, A.; Maneira, J.; Pedro, R.; Silva, J.; Delgado, A. Tavares] Univ Lisbon, Fac Ciencias, Lisbon, Portugal.
[Dos Santos, S. P. Amor; Carvalho, J.; Fiolhais, M. C. N.; Galhardo, B.; Veloso, F.; Wolters, H.] Univ Coimbra, Dept Phys, Coimbra, Portugal.
[Gomes, A.; Maio, A.; Saraiva, J. G.] Univ Lisbon, Ctr Fis Nucl, Lisbon, Portugal.
[Onofre, A.] Univ Minho, Dept Fis, Braga, Portugal.
[Aguilar-Saavedra, J. A.] Univ Granada, Dept Fis Teor & Cosmos, Granada, Spain.
[Aguilar-Saavedra, J. A.] Univ Granada, CAFPE, Granada, Spain.
Univ Nova Lisboa, Dep Fis, Caparica, Portugal.
Univ Nova Lisboa, CEFITEC, Fac Ciencias & Tecnol, Caparica, Portugal.
[Chudoba, J.; Havranek, M.; Hejbal, J.; Jakoubek, T.; Kepka, O.; Kupco, A.; Kus, V.; Lokajicek, M.; Lysak, R.; Marcisovsky, M.; Mikestikova, M.; Nemecek, S.; Penc, O.; Sicho, P.; Staroba, P.; Svatos, M.; Tasevsky, M.; Vrba, V.] Acad Sci Czech Republic, Inst Phys, Prague, Czech Republic.
[Berta, P.; Carli, I.; Davidek, T.; Dolejsi, J.; Dolezal, Z.; Kodys, P.; Kosek, T.; Leitner, R.; Reznicek, P.; Schaile, D.; Scheirich, D.; Slovak, R.; Spousta, M.; Sykora, T.; Tas, P.; Todorova-Nova, S.; Valkar, S.; Vorobel, V.] Charles Univ Prague, Fac Math & Phys, Prague, Czech Republic.
[Borisov, A.; Cheremushkina, E.; Denisov, S. P.; Fakhrutdinov, R. M.; Fenyuk, A. B.; Golubkov, D.; Kamenshchikov, A.; Karyukhin, A. N.; Kozhin, A. S.; Minaenko, A. A.; Myagkov, A. G.; Nikolaenko, V.; Ryzhov, A.; Solodkov, A. A.; Solovyanov, O. V.; Starchenko, E. A.; Vaniachine, A.; Zaitsev, A. M.; Zenin, O.] NRC KI, State Res Ctr Inst High Energy Phys Protvino, Protvino, Russia.
[Adye, T.; Baines, J. T.; Barnett, B. M.; Burke, S.; Dewhurst, A.; Dopke, J.; Emeliyanov, D.; Gallop, B. J.; Gee, C. N. P.; Haywood, S. J.; Kirk, J.; Martin-Haugh, S.; McMahon, S. J.; Middleton, R. P.; Murray, W. J.; Phillips, P. W.; Sankey, D. P. C.; Sawyer, C.; Tyndel, M.; Wickens, F. J.; Wielers, M.; Worm, S. D.] Rutherford Appleton Lab, Particle Phys Dept, Didcot, Oxon, England.
[Anulli, F.; Bagiacchi, P.; Bagnaia, P.; Bauce, M.; Bini, C.; Ciapetti, G.; Corradi, M.; De Pedis, D.; De Salvo, A.; Di Donato, C.; Falciano, S.; Gentile, S.; Giagu, S.; Gustavino, G.; Kuna, M.; Lacava, F.; Luci, C.; Luminari, L.; Messina, A.; Nisati, A.; Pasqualucci, E.; Petrolo, E.; Pontecorvo, L.; Rescigno, M.; Rosati, S.; Tehrani, F. Safai; Vanadia, M.; Vari, R.; Veneziano, S.; Verducci, M.; Zanello, L.] Ist Nazl Fis Nucl, Sez Roma, Rome, Italy.
[Bagiacchi, P.; Bagnaia, P.; Bauce, M.; Bini, C.; Ciapetti, G.; Corradi, M.; Di Donato, C.; Gentile, S.; Giagu, S.; Gustavino, G.; Kuna, M.; Lacava, F.; Luci, C.; Messina, A.; Vanadia, M.; Verducci, M.; Zanello, L.] Sapienza Univ Roma, Dipartimento Fis, Rome, Italy.
[Aielli, G.; Camarri, P.; Cardarelli, R.; Cerrito, L.; Di Ciaccio, A.; Iuppa, R.; Liberti, B.; Salamon, A.; Santonico, R.] Ist Nazl Fis Nucl, Sez Roma Tor Vergata, Rome, Italy.
[Aielli, G.; Camarri, P.; Cardarelli, R.; Cerrito, L.; Di Ciaccio, A.; Iuppa, R.; Liberti, B.; Salamon, A.; Santonico, R.] Univ Roma Tor Vergata, Dipartimento Fis, Rome, Italy.
[Baroncellia, A.; Biglietti, M.; Ceradini, F.; Di Micco, B.; Farilla, A.; Graziani, E.; Iodice, M.; Orestano, D.; Petrucci, F.; Puddu, D.; Salamanna, G.; Sessa, M.; Taccini, C.] Ist Nazl Fis Nucl, Sez Roma Tre, Rome, Italy.
[Ceradini, F.; Di Micco, B.; Orestano, D.; Petrucci, F.; Puddu, D.; Salamanna, G.; Sessa, M.; Taccini, C.] Univ Roma Tre, Dipartimento Matemat & Fis, Rome, Italy.
[Benchekroun, D.; Chafaq, A.; Hoummada, A.] Univ Hassan 2, Reseau Univ Phys Hautes Energies, Fac Sci Ain Chock, Casablanca, Morocco.
[Ghazlane, H.] Ctr Natl Energie Sci Tech Nucl, Rabat, Morocco.
[El Kacimi, M.; Goujdami, D.] Univ Cadi Ayyad, LPHEA Marrakech, Fac Sci Semlalia, Marrakech, Morocco.
[Aaboud, M.; Derkaoui, J. E.; Ouchrif, M.] Univ Mohamed Premier, Fac Sci, Oujda, Morocco.
[Aaboud, M.; Derkaoui, J. E.; Ouchrif, M.] LPTPM, Oujda, Morocco.
[El Moursli, R. Cherkaoui; Fassi, F.; Haddad, N.; Idrissi, Z.; Tayalati, Y.] Univ Mohammed 5, Fac Sci, Rabat, Morocco.
[Bachacou, H.; Balli, F.; Bauer, F.; Besson, N.; Blanchard, J. -B.; Boonekamp, M.; Chevalier, L.; Hoffmann, M. Dano; Deliot, F.; Denysiuk, D.; Etienvre, A. I.; Formica, A.; Pinto Firmino Da Costa, J. Goncalves; Guyot, C.; Jeanneau, F.; Kivernyk, O.; Lancon, E.; Laporte, J. F.; Le Quilleuc, E. P.; Lesage, A. A. J.; Mansoulie, B.; Meyer, J. -P.; Ouraou, A.; Rodriguez, L. Pacheco; Perego, M. M.; Peyaud, A.; Royon, C. R.; Saimpert, M.; Schoeffel, L.; Schwindling, J.] CEA Saclay Commissariat Energie Atom & Energies A, DSM IRFU Inst Rech Lois Fondamentales Univers, Gif Sur Yvette, France.
[AbouZeid, O. S.; Battaglia, M.; Debenedetti, C.; Grillo, A. A.; Hance, M.; Kuhl, A.; Law, A. T.; Litke, A. M.; Lockman, W. S.; Nielsen, J.; Reece, R.; Rose, P.; Sadrozinski, H. F. -W.; Schier, S.; Schumm, B. A.; Seiden, A.] Univ Calif Santa Cruz, Santa Cruz Inst Particle Phys, Santa Cruz, CA 95064 USA.
[Alpigiani, C.; Blackburn, D.; Goussiou, A. G.; Hsu, S. -C.; Johnson, W. J.; Lubatti, H. J.; Marx, M.; Meehan, S.; Rompotis, N.; Rosten, R.; Rothberg, J.; Russell, H. L.; De Bruin, P. H. Sales; Schaile, D.; Pastor, E. Torro; Watts, G.; Whallon, N. L.] Univ Washington, Dept Phys, Seattle, WA 98195 USA.
[Anastopoulos, C.; Costanzo, D.; Donszelmann, T. Cuhadar; Dawson, I.; Fletcher, G. T.; Hamity, G. N.; Hodgkinson, M. C.; Hodgson, P.; Johansson, P.; Klinger, J. A.; Korolkova, E. V.; Kyriazopoulos, D.; Paredes, B. Lopez; Macdonald, C. M.; Miyagawa, P. S.; Parker, K. A.; Schaile, D.; Tovey, D. R.; Vickey, T.; Boeriu, O. E. Vickey] Univ Sheffield, Dept Phys & Astron, Sheffield, S Yorkshire, England.
[Hasegawa, Y.; Takeshita, T.] Shinshu Univ, Dept Phys, Nagano, Japan.
[Atlay, N. B.; Buchholz, P.; Campoverde, A.; Czirr, H.; Fleck, I.; Ghasemi, S.; Ibragimov, I.; Li, Y.; Rosenthal, O.; Walkowiak, W.; Ziolkowski, M.] Univ Siegen, Fachbereich Phys, Siegen, Germany.
[Buat, Q.; Horton, A. J.; Mori, D.; O'Neil, D. C.; Pachal, K.; Stelzer, B.; Temple, D.; Torres, H.; Van Nieuwkoop, J.; Vetterli, M. C.] Simon Fraser Univ, Dept Phys, Burnaby, BC, Canada.
[Armbruster, A. J.; Barklow, T.; Bartoldus, R.; Bawa, H. S.; Black, J. E.; Gao, Y. S.; Garelli, N.; Grenier, P.; Ilic, N.; Kagan, M.; Kocian, M.; Koi, T.; Malone, C.; Moss, J.; Mount, R.; Nachman, B. P.; Piacquadio, G.; Rubbo, F.; Salnikov, A.; Schwartzman, A.; Su, D.; Tompkins, L.; Wittgen, M.; Young, C.; Zeng, Q.] SLAC Natl Accelerator Lab, Stanford, CA USA.
[Astalos, R.; Bartos, P.; Blazek, T.; Dado, T.; Melo, M.; Plazak, L.; Smiesko, J.; Sykora, I.; Tokar, S.; Zenis, T.] Comenius Univ, Fac Math Phys & Informat, Bratislava, Slovakia.
[Bruncko, D.; Kladivab, E.; Strizenecb, P.; Urban, J.] Slovak Acad Sci, Inst Expt Phys, Dept Subnucl Phys, Kosice, Slovakia.
[Castaneda-Miranda, E.; Hamilton, A.; Yacoob, S.] Univ Cape Town, Dept Phys, Cape Town, South Africa.
[Connell, S. H.; Govender, N.] Univ Johannesburg, Dept Phys, Johannesburg, South Africa.
[Hsuc, C.; Karc, D.; Garciac, B. R. Mellado; Ruan, X.] Univ Witwatersrand, Sch Phys, Johannesburg, South Africa.
[Abulaiti, Y.; Akerstedt, H.; Asman, B.; Bendtz, K.; Bertoli, G.; Bylund, O. Bessidskaia; Bohm, C.; Clement, C.; Cribbs, W. A.; Hellman, S.; Jon-And, K.; Lundberg, O.; Milstead, D. A.; Moa, T.; Molander, S.; Pani, P.; Poettgen, R.; Rossetti, V.; Shaikh, N. W.; Shcherbakova, A.; Silverstein, S. B.; Sjolin, J.; Strandberg, S.; Ughetto, M.; Santurio, E. Valdes; Wallangen, V.] Stockholm Univ, Dept Phys, Stockholm, Sweden.
[Abulaiti, Y.; Akerstedt, H.; Asman, B.; Bendtz, K.; Bertoli, G.; Bylund, O. Bessidskaia; Clement, C.; Cribbs, W. A.; Hellman, S.; Jon-And, K.; Lundberg, O.; Milstead, D. A.; Moa, T.; Molander, S.; Pani, P.; Poettgen, R.; Rossetti, V.; Shaikh, N. W.; Shcherbakova, A.; Sjolin, J.; Strandberg, S.; Ughetto, M.; Santurio, E. Valdes; Wallangen, V.] Oskar Klein Ctr, Stockholm, Sweden.
[Lund-Jensen, B.; Sidebo, P. E.; Strandberg, J.] Royal Inst Technol, Dept Phys, Stockholm, Sweden.
[Backes, M.; Balestri, T.; Bee, C. P.; Chen, K.; Hobbs, J.; Huo, P.; Jia, J.; Li, H.; Lindquist, B. E.; McCarthy, R. L.; Montalbano, A.; Morvaj, L.; Radhakrishnan, S. K.; Rijssenbeek, M.; Schamberger, R. D.; Tsybychev, D.; Zaman, A.; Zhou, M.] SUNY Stony Brook, Dept Phys & Astron, Stony Brook, NY 11794 USA.
[Backes, M.; Balestri, T.; Bee, C. P.; Chen, K.; Hobbs, J.; Huo, P.; Jia, J.; Li, H.; Lindquist, B. E.; McCarthy, R. L.; Montalbano, A.; Morvaj, L.; Radhakrishnan, S. K.; Rijssenbeek, M.; Schaile, D.; Schamberger, R. D.; Tsybychev, D.; Zaman, A.; Zhou, M.] SUNY Stony Brook, Dept Chem, Stony Brook, NY 11794 USA.
[Abraham, N. L.; Allbrooke, B. M. M.; Asquith, L.; Cerri, A.; Barajas, C. A. Chavez; De Sanctis, U.; De Santo, A.; Lerner, G.; Miano, F.; Salvatore, F.; Castillo, I. Santoyo; Shehu, C. Y.; Suruliz, K.; Sutton, M. R.; Vivarelli, I.; Winston, O. J.] Univ Sussex, Dept Phys & Astron, Brighton, E Sussex, England.
[Black, C. W.; Finelli, K. D.; Jeng, G. -Y.; Limosani, A.; Morley, A. K.; Saavedra, A. F.; Scarcella, M.; Varvell, K. E.; Wang, J.; Yabsley, B.] Univ Sydney, Sch Phys, Sydney, NSW, Australia.
[Hou, S.; Hsu, P. J.; Lee, S. C.; Lin, S. C.; Liu, B.; Liu, D.; LoSterzo, F.; Mazini, R.; Shi, L.; Soh, D. A.; Teng, P. K.; Wang, S. M.; Yang, Y.] Acad Sinica, Inst Phys, Taipei, Taiwan.
[Abreu, H.; Gozani, E.; Rozen, Y.; Tarem, S.; van Eldik, N.] Technion Israel Inst Technol, Dept Phys, Haifa, Israel.
[Abramowicz, H.; Alexander, G.; Ashkenazi, A.; Bella, G.; Benary, O.; Benhammou, Y.; Davies, M.; Duarte-Campderros, J.; Etzion, E.; Gershon, A.; Gueta, O.; Oren, Y.; Soffer, A.; Taiblum, N.] Tel Aviv Univ, Raymond & Beverly Sackler Sch Phys & Astron, Tel Aviv, Israel.
[Gentsos, C.; Gkaitatzis, S.; Gkialas, I.; Iliadis, D.; Kimura, N.; Kordas, K.; Leisos, A.; Papageorgiou, K.; Petridou, C.; Sampsonidis, D.] Aristotle Univ Thessaloniki, Dept Phys, Thessaloniki, Greece.
[Asai, S.; Chen, S.; Enari, Y.; Hanawa, K.; Ishino, M.; Kanaya, N.; Kataoka, Y.; Kato, C.; Kawamoto, T.; Kishimoto, T.; Kobayashi, A.; Kobayashi, T.; Komori, Y.; Kozakai, C.; Mashimo, T.; Masubuchi, T.; Minami, Y.; Mori, T.; Morinaga, M.; Nakamura, T.; Ninomiya, Y.; Nobe, T.; Okumura, Y.; Saito, T.; Sakamoto, H.; Sasaki, Y.; Tanaka, J.; Terashi, K.; Ueda, I.; Yamamoto, S.; Yamanaka, T.] Univ Tokyo, Int Ctr Elementary Particle Phys, Tokyo, Japan.
[Asai, S.; Chen, S.; Enari, Y.; Hanawa, K.; Ishino, M.; Kanaya, N.; Kataoka, Y.; Kato, C.; Kawamoto, T.; Kishimoto, T.; Kobayashi, A.; Kobayashi, T.; Komori, Y.; Kozakai, C.; Mashimo, T.; Masubuchi, T.; Minami, Y.; Mori, T.; Morinaga, M.; Nakamura, T.; Ninomiya, Y.; Nobe, T.; Okumura, Y.; Saito, T.; Sakamoto, H.; Tanaka, J.; Terashi, K.; Ueda, I.; Yamamoto, S.; Yamanaka, T.] Univ Tokyo, Dept Phys, Tokyo, Japan.
[Bratzler, U.; Fukunaga, C.] Tokyo Metropolitan Univ, Grad Sch Sci & Technol, Tokyo, Japan.
[Hayakawa, D.; Ishitsuka, M.; Jinnouchi, O.; Kobayashi, D.; Kuze, M.; Motohashi, K.; Tanaka, M.; Todome, K.; Yamaguchi, D.] Tokyo Inst Technol, Dept Phys, Tokyo, Japan.
[Batista, S. J.; Chau, C. C.; Cormier, K. J. R.; DeMarco, D. A.; Di Sipio, R.; Diamond, M.; Keoshkerian, H.; Krieger, P.; Liblong, A.; Mc Goldrick, G.; Orr, R. S.; Pascuzzi, V. R.; Polifka, R.; Rudolph, M. S.; Savard, P.; Sinervo, P.; Taenzer, J.; Teuscher, R. J.; Trischuk, W.; Veloce, L. M.; Venturi, N.] Univ Toronto, Dept Phys, Toronto, ON, Canada.
[Canepa, A.; Chekulaev, S. V.; Hod, N.; Jovicevic, J.; Codina, E. Perez; Schneider, B.; Stelzer-Chilton, O.; Tafirout, R.; Trigger, I. M.] TRIUMF, Vancouver, BC, Canada.
[Ramos, J. Manjarres; Palacino, G.; Taylor, W.] York Univ, Dept Phys & Astron, Toronto, ON, Canada.
[Hara, K.; Ito, F.; Kasahara, K.; Kim, S. H.; Kiuchi, K.; Nagata, K.; Okawa, H.; Sato, K.; Ukegawa, F.] Univ Tsukuba, Fac Pure & Appl Sci, Tsukuba, Ibaraki, Japan.
[Hara, K.; Ito, F.; Kasahara, K.; Kim, S. H.; Kiuchi, K.; Nagata, K.; Okawa, H.; Sato, K.; Ukegawa, F.] Univ Tsukuba, Ctr Integrated Res Fundamental Sci & Engn, Tsukuba, Ibaraki, Japan.
[Beauchemin, P. H.; Meoni, E.; Sliwa, K.; Son, H.; Wetter, J.] Tufts Univ, Dept Phys & Astron, Medford, MA USA.
[Casper, D. W.; Corso-Radu, A.; Frate, M.; Guest, D.; Lankford, A. J.; Mete, A. S.; Nelson, A.; Neubauer, M. S.; Scannicchio, D. A.; Schaile, D.; Schernau, M.; Shimmin, C. O.; Taffard, A.; Unel, G.; Whiteson, D.] Univ Calif Irvine, Dept Phys & Astron, Irvine, CA USA.
[Acharya, B. S.; Boldyrev, A. S.; Cobal, M.; Giordani, M. P.; Pinamonti, M.; Quayle, W. B.; Schaile, D.; Serkin, L.; Shaw, K.; Soualah, R.; Truong, L.] Ist Nazl Fis Nucl, Grp Collegato Udine, Sez Trieste, Udine, Italy.
[Acharya, B. S.; Quayle, W. B.; Serkin, L.; Shaw, K.] Abdus Salaam Int Ctr Theoret Phys, Trieste, Italy.
[Boldyrev, A. S.; Cobal, M.; Giordani, M. P.; Pinamonti, M.; Soualah, R.; Truong, L.] Univ Udine, Dipartimento Chim Fis & Ambiente, Udine, Italy.
[Kuutmann, E. Bergeaas; Brenner, R.; Ekelof, T.; Ellert, M.; Ferrari, A.; Maddocks, H. J.; Ohman, H.; Rangel-Smith, C.] Uppsala Univ, Dept Phys & Astron, Uppsala, Sweden.
[Atkinson, M.; Armadans, R. Caminal; Cavaliere, V.; Chang, P.; Errede, S.; Hooberman, B. H.; Khader, M.; Lie, K.; Liss, T. M.; Liu, L.; Long, J. D.; Outschoorn, V. I. Martinez; Rybar, M.; Shang, R.; Sickles, A. M.; Vichou, I.; Zeng, J. C.] Univ Illinois, Dept Phys, 1110 W Green St, Urbana, IL 61801 USA.
[Piqueras, D. Alvarez; Navarro, L. Barranco; Urban, S. Cabrera; Gimenez, V. Castillo; Alberich, L. Cerda; Costa, M. J.; Martinez, P. Fernandez; Ferrer, A.; Fiorini, L.; Fuster, J.; Garcia, C.; Navarro, J. E. Garcia; de la Hoz, S. Gonzalez; Jimenez, Y. Hernandez; Higon-Rodriguez, E.; Pena, J. Jimenez; King, M.; Lacasta, C.; Lacuesta, V. R.; Mamuzic, J.; Marti-Garcia, S.; Melini, D.; Mitsou, V. A.; Lopez, S. Pedraza; Rodriguez, D. Rodriguez; Adam, E. Romero; Ros, E.; Salt, J.; Sanchez, J.; Martinez, V. Sanchez; Soldevila, U.; Valero, A.; Ferrer, J. A. Valls; Vos, M.] Univ Valencia, Inst Fis Corpuscular IFIC, Valencia, Spain.
[Piqueras, D. Alvarez; Navarro, L. Barranco; Urban, S. Cabrera; Gimenez, V. Castillo; Alberich, L. Cerda; Costa, M. J.; Martinez, P. Fernandez; Ferrer, A.; Fiorini, L.; Fuster, J.; Garcia, C.; Navarro, J. E. Garcia; de la Hoz, S. Gonzalez; Jimenez, Y. Hernandez; Higon-Rodriguez, E.; Pena, J. Jimenez; King, M.; Lacasta, C.; Lacuesta, V. R.; Mamuzic, J.; Marti-Garcia, S.; Melini, D.; Mitsou, V. A.; Lopez, S. Pedraza; Rodriguez, D. Rodriguez; Adam, E. Romero; Ros, E.; Salt, J.; Sanchez, J.; Martinez, V. Sanchez; Schaile, D.; Soldevila, U.; Valero, A.; Ferrer, J. A. Valls; Vos, M.] Univ Valencia, Dept Fis Atom Mol & Nucl, Valencia, Spain.
[Piqueras, D. Alvarez; Navarro, L. Barranco; Urban, S. Cabrera; Gimenez, V. Castillo; Alberich, L. Cerda; Costa, M. J.; Martinez, P. Fernandez; Ferrer, A.; Fiorini, L.; Fuster, J.; Garcia, C.; Navarro, J. E. Garcia; de la Hoz, S. Gonzalez; Jimenez, Y. Hernandez; Higon-Rodriguez, E.; Pena, J. Jimenez; King, M.; Lacasta, C.; Lacuesta, V. R.; Mamuzic, J.; Marti-Garcia, S.; Melini, D.; Mitsou, V. A.; Lopez, S. Pedraza; Rodriguez, D. Rodriguez; Adam, E. Romero; Ros, E.; Salt, J.; Sanchez, J.; Martinez, V. Sanchez; Soldevila, U.; Valero, A.; Ferrer, J. A. Valls; Vos, M.] Univ Valencia, Dept Ingn Elect, Valencia, Spain.
[Piqueras, D. Alvarez; Navarro, L. Barranco; Urban, S. Cabrera; Gimenez, V. Castillo; Alberich, L. Cerda; Costa, M. J.; Martinez, P. Fernandez; Ferrer, A.; Fiorini, L.; Fuster, J.; Garcia, C.; Navarro, J. E. Garcia; de la Hoz, S. Gonzalez; Jimenez, Y. Hernandez; Higon-Rodriguez, E.; Pena, J. Jimenez; King, M.; Lacasta, C.; Lacuesta, V. R.; Mamuzic, J.; Marti-Garcia, S.; Melini, D.; Mitsou, V. A.; Lopez, S. Pedraza; Rodriguez, D. Rodriguez; Adam, E. Romero; Ros, E.; Salt, J.; Sanchez, J.; Martinez, V. Sanchez; Soldevila, U.; Valero, A.; Ferrer, J. A. Valls; Vos, M.] Univ Valencia, Inst Microelect Barcelona IMB CNM, Valencia, Spain.
[Piqueras, D. Alvarez; Navarro, L. Barranco; Urban, S. Cabrera; Gimenez, V. Castillo; Alberich, L. Cerda; Costa, M. J.; Martinez, P. Fernandez; Ferrer, A.; Fiorini, L.; Fuster, J.; Garcia, C.; Navarro, J. E. Garcia; de la Hoz, S. Gonzalez; Jimenez, Y. Hernandez; Higon-Rodriguez, E.; Pena, J. Jimenez; King, M.; Lacasta, C.; Lacuesta, V. R.; Mamuzic, J.; Marti-Garcia, S.; Melini, D.; Mitsou, V. A.; Lopez, S. Pedraza; Rodriguez, D. Rodriguez; Adam, E. Romero; Ros, E.; Salt, J.; Sanchez, J.; Martinez, V. Sanchez; Schaile, D.; Schamberger, R. D.; Soldevila, U.; Valero, A.; Ferrer, J. A. Valls; Vos, M.] CSIC, Valencia, Spain.
[Danninger, M.; Fedorko, W.; Gay, C.; Gecse, Z.; Gignac, M.; Henkelmann, S.; King, S. B.; Lister, A.] Univ British Columbia, Dept Phys, Vancouver, BC, Canada.
[Albert, J.; David, C.; Elliot, A. A.; Fincke-Keeler, M.; Hamano, K.; Hill, E.; Keeler, R.; Kowalewski, R.; Kuwertz, E. S.; Kwan, T.; LeBlanc, M.; Lefebvre, M.; McPherson, R. A.; Pearce, J.; Seuster, R.; Sobie, R.; Trovatelli, M.; Venturi, M.] Univ Victoria, Dept Phys & Astron, Victoria, BC, Canada.
[Beckingham, M.; Ennis, J. S.; Farrington, S. M.; Harrison, P. F.; Jeske, C.; Jones, G.; Martin, T. A.; Murray, W. J.; Pianori, E.; Spangenberg, M.] Univ Warwick, Dept Phys, Coventry, W Midlands, England.
[Iizawa, T.; Kaji, T.; Mitani, T.; Sakurai, Y.; Yorita, K.] Waseda Univ, Tokyo, Japan.
[Balek, P.; Bressler, S.; Citron, Z. H.; Duchovni, E.; Dumancic, M.; Gross, E.; Kohler, M. K.; Lellouch, D.; Levinson, L. J.; Mikenberg, G.; Milov, A.; Pitt, M.; Ravinovich, I.; Roth, I.; Schaarschmidt, J.; Schaile, D.; Smakhtin, V.; Turgeman, D.] Weizmann Inst Sci, Dept Particle Phys, Rehovot, Israel.
[Banerjee, Sw.; Guan, W.; Hard, A. S.; Heng, Y.; Ju, X.; Kaplan, L. S.; Kashif, L.; Kruse, A.; Ming, Y.; Wang, F.; Wiedenmann, W.; Wu, S. L.; Yang, H.; Zhang, F.; Zobernig, G.] Univ Wisconsin, Dept Phys, 1150 Univ Ave, Madison, WI 53706 USA.
[Herget, V.; Kuger, F.; Redelbach, A.; Schreyer, M.; Sidiropoulou, O.; Siragusa, G.; Stroehmer, R.; Trefzger, T.; Weber, S. W.; Zibell, A.] Julius Maximilians Univ, Fak Phys & Astron, Wurzburg, Germany.
[Bannoura, A. A. E.; Boerner, D.; Braun, H. M.; Cornelissen, T.; Ellinghaus, F.; Ernis, G.; Fischer, J.; Flick, T.; Gabizon, O.; Gilles, G.; Hamacher, K.; Harenberg, T.; Hirschbuehl, D.; Kersten, S.; Kuechler, J. T.; Maettig, P.; Neumann, M.; Pataraia, S.; Riegel, C. J.; Sandhoff, M.; Tepel, F.; Vogel, M.; Wagner, W.; Zeitnitz, C.] Berg Univ Wuppertal, Fak Math & Nat Wissensch, Fachgrp Phys, Wuppertal, Germany.
[Baker, O. K.; Noccioli, E. Benhar; Cummings, J.; Demers, S.; Ideal, E.; Lagouri, T.; Leister, A. G.; Loginov, A.; Hernandez, D. Paredes; Thomsen, L. A.; Tipton, P.; Vasquez, J. G.; Wang, X.] Yale Univ, Dept Phys, New Haven, CT USA.
[Hakobyan, H.; Vardanyan, G.] Yerevan Phys Inst, Yerevan, Armenia.
[Rahal, G.] IN2P3, Ctr Calcul, Villeurbanne, France.
[Acharya, B. S.] Kings Coll London, Dept Phys, London, England.
[Ahmadov, F.; Huseynov, N.; Javadov, N.] Azerbaijan Acad Sci, Inst Phys, Baku, Azerbaijan.
[Anisenkov, A. V.; Baldin, E. M.; Bobrovnikov, V. S.; Buzykaev, A. R.; Kazanin, V. F.; Kharlamov, A. G.; Korol, A. A.; Maslennikov, A. L.; Maximov, D. A.; Peleganchuk, S. V.; Rezanova, O. L.; Schaile, D.; Soukharev, A. M.; Talyshev, A. A.; Tikhonov, Yu. A.] Novosibirsk State Univ, Novosibirsk, Russia.
[Azuelos, G.; Gingrich, D. M.; Oakham, F. G.; Savard, P.; Vetterli, M. C.] TRIUMF, Vancouver, BC, Canada.
[Banerjee, Sw.] Univ Louisville, Dept Phys & Astron, Louisville, KY 40292 USA.
[Bawa, H. S.; Gao, Y. S.] Calif State Univ Fresno, Dept Phys, Fresno, CA 93740 USA.
[Beck, H. P.] Univ Fribourg, Dept Phys, Fribourg, Switzerland.
[Casado, M. P.] Univ Autonoma Barcelona, Dept Fis, Barcelona, Spain.
[Castro, N. F.] Univ Porto, Dept Fis & Astron, Fac Ciencias, Oporto, Portugal.
[Chelkov, G. A.] Tomsk State Univ, Tomsk, Russia.
[Conventi, F.; Della Pietra, M.] Univ Napoli Parthenope, Naples, Italy.
[Corriveau, F.; McPherson, R. A.; Robertson, S. H.; Sobie, R.; Teuscher, R. J.] Inst Particle Phys IPP, Victoria, BC, Canada.
[Ducu, O. A.] Natl Inst Phys & Nucl Engn, Bucharest, Romania.
[Fedin, O. L.] St Petersburg State Polytech Univ, Dept Phys, St Petersburg, Russia.
[Geng, C.; Guo, Y.; Li, B.] Univ Michigan, Dept Phys, Ann Arbor, MI USA.
[Govender, N.] Ctr High Performance Comp, CSIR Campus, Cape Town, South Africa.
[Greenwood, Z. D.; Sawyer, L.] Louisiana Tech Univ, Ruston, LA 71270 USA.
[Grinstein, S.; Rozas, A. Juste; Martinez, M.] ICREA, Barcelona, Spain.
[Hanagaki, K.] Osaka Univ, Grad Sch Sci, Osaka, Japan.
[Hsu, P. J.] Natl Tsing Hua Univ, Dept Phys, Hsinchu, Taiwan.
[Igonkina, O.] Radboud Univ Nijmegen Nikhef, Inst Math Astrophys & Particle Phys, Nijmegen, Netherlands.
[Ilchenko, Y.; Onyisi, P. U. E.] Univ Texas Austin, Dept Phys, Austin, TX 78712 USA.
[Jejelava, J.] Ilia State Univ, Inst Theoret Phys, Tbilisi, Rep of Georgia.
[Jenni, P.] CERN, Geneva, Switzerland.
[Khubua, J.] Georgian Tech Univ GTU, Tbilisi, Rep of Georgia.
[Kono, T.; Nagai, R.] Ochanomizu Univ, Ochadai Acad Prod, Tokyo, Japan.
[Konoplich, R.] Manhattan Coll, New York, NY USA.
[Leisos, A.] Hellen Open Univ, Patras, Greece.
[Lin, S. C.] Acad Sinica, Acad Sinica Grid Comp, Inst Phys, Taipei, Taiwan.
[Liu, B.] Shandong Univ, Sch Phys, Jinan, Shandong, Peoples R China.
[Myagkov, A. G.; Nikolaenko, V.; Zaitsev, A. M.] State Univ, Moscow Inst Phys & Technol, Dolgoprudnyi, Russia.
[Nessi, M.] Univ Geneva, Sect Phys, Geneva, Switzerland.
[Pasztor, G.] Eotvos Lorand Univ, Budapest, Hungary.
[Piacquadio, G.] SUNY Stony Brook, Dept Phys & Astron, Stony Brook, NY 11794 USA.
[Piacquadio, G.] SUNY Stony Brook, Dept Chem, Stony Brook, NY 11794 USA.
[Pinamonti, M.] Int Sch Adv Studies SISSA, Trieste, Italy.
[Purohit, M.] Univ S Carolina, Dept Phys & Astron, Columbia, SC 29208 USA.
[Shi, L.] Sun Yat Sen Univ, Sch Phys & Engn, Guangzhou, Guangdong, Peoples R China.
[Shiyakova, M.] Bulgarian Acad Sci, Inst Nucl Res & Nucl Energy INRNE, Sofia, Bulgaria.
[Smirnova, L. N.] Moscow MV Lomonosov State Univ, Fac Phys, Moscow, Russia.
[Song, H. Y.; Zhang, G.] Acad Sinica, Inst Phys, Taipei, Taiwan.
[Tikhomirov, V. O.] Natl Res Nucl Univ MEPhI, Moscow, Russia.
[Tompkins, L.] Stanford Univ, Dept Phys, Stanford, CA 94305 USA.
[Toth, J.] Wigner Res Ctr Phys, Inst Particle & Nucl Phys, Budapest, Hungary.
[Vest, A.] Flensburg Univ Appl Sci, Flensburg, Germany.
[Yusuff, I.] Univ Malaya, Dept Phys, Kuala Lumpur, Malaysia.
[Zhang, R.] Aix Marseille Univ, CPPM, Marseille, France.
[Zhang, R.] CNRS IN2P3, Marseille, France.
RP Aaboud, M (reprint author), Univ Mohamed Premier, Fac Sci, Oujda, Morocco.; Aaboud, M (reprint author), LPTPM, Oujda, Morocco.
RI Li, Liang/O-1107-2015; Monzani, Simone/D-6328-2017; Warburton,
Andreas/N-8028-2013; Tikhomirov, Vladimir/M-6194-2015; Kuday,
Sinan/C-8528-2014; Gladilin, Leonid/B-5226-2011; Mitsou,
Vasiliki/D-1967-2009; Camarri, Paolo/M-7979-2015; Carvalho,
Joao/M-4060-2013; Prokoshin, Fedor/E-2795-2012; Yang,
Haijun/O-1055-2015; Solodkov, Alexander/B-8623-2017; Doyle,
Anthony/C-5889-2009; Zaitsev, Alexandre/B-8989-2017; Leitner,
Rupert/C-2004-2017; Carli, Ina/C-2189-2017; messina, andrea/C-2753-2013;
Guo, Jun/O-5202-2015; Livan, Michele/D-7531-2012; Villa,
Mauro/C-9883-2009; Peleganchuk, Sergey/J-6722-2014
OI Li, Liang/0000-0001-6411-6107; Monzani, Simone/0000-0002-0479-2207;
Warburton, Andreas/0000-0002-2298-7315; Tikhomirov,
Vladimir/0000-0002-9634-0581; Kuday, Sinan/0000-0002-0116-5494;
Gladilin, Leonid/0000-0001-9422-8636; Mitsou,
Vasiliki/0000-0002-1533-8886; Camarri, Paolo/0000-0002-5732-5645;
Carvalho, Joao/0000-0002-3015-7821; Prokoshin,
Fedor/0000-0001-6389-5399; Solodkov, Alexander/0000-0002-2737-8674;
Doyle, Anthony/0000-0001-6322-6195; Zaitsev,
Alexandre/0000-0002-4961-8368; Leitner, Rupert/0000-0002-2994-2187;
Carli, Ina/0000-0002-0411-1141; Guo, Jun/0000-0001-8125-9433; Livan,
Michele/0000-0002-5877-0062; Villa, Mauro/0000-0002-9181-8048;
Peleganchuk, Sergey/0000-0003-0907-7592
FU ANPCyT, Argentina; YerPhI, Armenia; ARC, Australia; BMWFW, Austria; FWF,
Austria; ANAS, Azerbaijan; SSTC, Belarus; CNPq, Brazil; FAPESP, Brazil;
NSERC, Canada; NRC, Canada; CFI, Canada; CERN; CONICYT, Chile; CAS,
China; MOST, China; NSFC, China; COLCIENCIAS, Colombia; MSMT CR, Czech
Republic; MPO CR, Czech Republic; VSC CR, Czech Republic; DNRF, Denmark;
DNSRC, Denmark; IN2P3-CNRS, France; CEA-DSM/IRFU, France; GNSF, Georgia;
BMBF, Germany; HGF, Germany; MPG, Germany; GSRT, Greece; RGC, Hong Kong
SAR, China; ISF, Israel; I-CORE, Israel; Benoziyo Center, Israel; INFN,
Italy; MEXT, Japan; JSPS, Japan; CNRST, Morocco; FOM, Netherlands; NWO,
Netherlands; RCN, Norway; MNiSW, Poland; NCN, Poland; FCT, Portugal;
MNE/IFA, Romania; MES of Russia; NRC KI, Russian Federation; JINR;
MESTD, Serbia; MSSR, Slovakia; ARRS, Slovenia; MIZS, Slovenia; DST/NRF,
South Africa; MINECO, Spain; SRC, Sweden; Wallenberg Foundation, Sweden;
SERI, Switzerland; SNSF, Switzerland; Cantons of Bern and Geneva,
Switzerland; MOST, Taiwan; TAEK, Turkey; STFC, United Kingdom; DOE,
United States of America; NSF, United States of America; BCKDF; Canada
Council; CANARIE; CRC; Compute Canada; FQRNT; Ontario InnovationTrust,
Canada; EPLANET; ERC; FP7; Marie Sklodowska-Curie Actions, European
Union; Investissements d'Avenir Labex and Idex, France; ANR, France;
Region Auvergne, France; Fondation Partager le Savoir, France; DFG,
Germany; AvH Foundation, Germany; EU-ESF; Greek NSRF; BSF, Israel; GIF,
Israel; Minerva, Israel; BRF, Norway; Generalitat de Catalunya, Spain;
Generalitat Valenciana, Spain; Royal Society, United Kingdom; Leverhulme
Trust, United Kingdom
FX We thank CERN for the very successful operation of the LHC, as well as
the support staff from our institutions without whom ATLAS could not be
operated efficiently. We acknowledge the support of ANPCyT, Argentina;
YerPhI, Armenia; ARC, Australia; BMWFW and FWF, Austria; ANAS,
Azerbaijan; SSTC, Belarus; CNPq and FAPESP, Brazil; NSERC, NRC and CFI,
Canada; CERN; CONICYT, Chile; CAS, MOST and NSFC, China; COLCIENCIAS,
Colombia; MSMT CR, MPO CR and VSC CR, Czech Republic; DNRF and DNSRC,
Denmark; IN2P3-CNRS, CEA-DSM/IRFU, France; GNSF, Georgia; BMBF, HGF, and
MPG, Germany; GSRT, Greece; RGC, Hong Kong SAR, China; ISF, I-CORE and
Benoziyo Center, Israel; INFN, Italy; MEXT and JSPS, Japan; CNRST,
Morocco; FOM and NWO, Netherlands; RCN, Norway; MNiSW and NCN, Poland;
FCT, Portugal; MNE/IFA, Romania; MES of Russia and NRC KI, Russian
Federation; JINR; MESTD, Serbia; MSSR, Slovakia; ARRS and MIZS,
Slovenia; DST/NRF, South Africa; MINECO, Spain; SRC and Wallenberg
Foundation, Sweden; SERI, SNSF and Cantons of Bern and Geneva,
Switzerland; MOST, Taiwan; TAEK, Turkey; STFC, United Kingdom; DOE and
NSF, United States of America. In addition, individual groups and
members have received support from BCKDF, the Canada Council, CANARIE,
CRC, Compute Canada, FQRNT, and the Ontario InnovationTrust, Canada;
EPLANET, ERC, FP7, Horizon 2020 and Marie Sklodowska-Curie Actions,
European Union; Investissements d'Avenir Labex and Idex, ANR, Region
Auvergne and Fondation Partager le Savoir, France; DFG and AvH
Foundation, Germany; Herakleitos, Thales and Aristeia programmes
co-financed by EU-ESF and the Greek NSRF; BSF, GIF and Minerva, Israel;
BRF, Norway; Generalitat de Catalunya, Generalitat Valenciana, Spain;
the Royal Society and Leverhulme Trust, United Kingdom. The crucial
computing support from all WLCG partners is acknowledged gratefully, in
particular from CERN, the ATLAS Tier-1 facilities at TRIUMF (Canada),
NDGF (Denmark, Norway, Sweden), CC-IN2P3 (France), KIT/GridKA (Germany),
INFN-CNAF (Italy), NL-T1 (Netherlands), PIC (Spain), ASGC (Taiwan), RAL
(UK) and BNL (USA), the Tier-2 facilities worldwide and large non-WLCG
resource providers. Major contributors of computing resources are listed
in Ref. [83].
NR 82
TC 2
Z9 2
U1 25
U2 25
PU SPRINGER
PI NEW YORK
PA 233 SPRING ST, NEW YORK, NY 10013 USA
SN 1434-6044
EI 1434-6052
J9 EUR PHYS J C
JI Eur. Phys. J. C
PD OCT 6
PY 2016
VL 76
IS 10
AR 547
DI 10.1140/epjc/s10052-016-4382-4
PG 25
WC Physics, Particles & Fields
SC Physics
GA DY6PJ
UT WOS:000385249500004
PM 28316487
ER
PT J
AU Hehn, L
Armengaud, E
Arnaud, Q
Augier, C
Benoit, A
Berge, L
Billard, J
Blumer, J
de Boissiere, T
Broniatowski, A
Camus, P
Cazes, A
Chapellier, M
Charlieux, F
De Jesus, M
Dumoulin, L
Eitel, K
Foerster, N
Gascon, J
Giuliani, A
Gros, M
Heuermann, G
Jin, Y
Juillard, A
Kefelian, C
Kleifges, M
Kozlov, V
Kraus, H
Kudryavtsev, VA
Le-Sueur, H
Marnieros, S
Navick, XF
Nones, C
Olivieri, E
Pari, P
Paul, B
Piro, MC
Poda, D
Queguiner, E
Rozov, S
Sanglard, V
Schmidt, B
Scorza, S
Siebenborn, B
Tcherniakhovski, D
Vagneron, L
Weber, M
Yakushev, E
AF Hehn, L.
Armengaud, E.
Arnaud, Q.
Augier, C.
Benoit, A.
Berge, L.
Billard, J.
Bluemer, J.
de Boissiere, T.
Broniatowski, A.
Camus, P.
Cazes, A.
Chapellier, M.
Charlieux, F.
De Jesus, M.
Dumoulin, L.
Eitel, K.
Foerster, N.
Gascon, J.
Giuliani, A.
Gros, M.
Heuermann, G.
Jin, Y.
Juillard, A.
Kefelian, C.
Kleifges, M.
Kozlov, V.
Kraus, H.
Kudryavtsev, V. A.
Le-Sueur, H.
Marnieros, S.
Navick, X. -F.
Nones, C.
Olivieri, E.
Pari, P.
Paul, B.
Piro, M. -C.
Poda, D.
Queguiner, E.
Rozov, S.
Sanglard, V.
Schmidt, B.
Scorza, S.
Siebenborn, B.
Tcherniakhovski, D.
Vagneron, L.
Weber, M.
Yakushev, E.
TI Improved EDELWEISS-III sensitivity for low-mass WIMPs using a profile
likelihood approach
SO EUROPEAN PHYSICAL JOURNAL C
LA English
DT Article
ID DARK-MATTER; SEARCH
AB We report on a dark matter search for a Weakly Interacting Massive Particle (WIMP) in the mass range m(chi) is an element of [4, 30] GeV/c(2) with the EDELWEISS-III experiment. A 2D profile likelihood analysis is performed on data from eight selected detectors with the lowest energy thresholds leading to a combined fiducial exposure of 496 kg-days. External backgrounds from gamma- and beta-radiation, recoils from Pb-206 and neutrons as well as detector intrinsic backgrounds were modelled from data outside the region of interest and constrained in the analysis. The basic data selection and most of the background models are the same as those used in a previously published analysis based on boosted decision trees (BDT) [1]. For the likelihood approach applied in the analysis presented here, a larger signal efficiency and a subtraction of the expected background lead to a higher sensitivity, especially for the lowest WIMP masses probed. No statistically significant signal was found and upper limits on the spin-independent WIMP-nucleon scattering cross section can be set with a hypothesis test based on the profile likelihood test statistics. The 90 % C.L. exclusion limit set for WIMPs with m(chi) = 4 GeV/c(2) is 1.6 x 10(-39) cm(2), which is an improvement of a factor of seven with respect to the BDT-based analysis. For WIMP masses above 15 GeV/c(2) the exclusion limits found with both analyses are in good agreement.
C1 [Hehn, L.; Bluemer, J.; Eitel, K.; Kozlov, V.; Schmidt, B.; Siebenborn, B.] Karlsruhe Inst Technol, Inst Kernphys, Postfach 3640, D-76021 Karlsruhe, Germany.
[Armengaud, E.; de Boissiere, T.; Gros, M.; Navick, X. -F.; Nones, C.; Paul, B.] CEA Saclay, DSM IRFU, F-91191 Gif Sur Yvette, France.
[Augier, C.; Billard, J.; Cazes, A.; Charlieux, F.; De Jesus, M.; Gascon, J.; Juillard, A.; Kefelian, C.; Queguiner, E.; Sanglard, V.; Vagneron, L.] Univ Lyon 1, CNRS, Inst Phys Nucl Lyon, IN2P3, 4 Rue Enrico Fermi, F-69622 Lyon, France.
[Benoit, A.; Camus, P.] UJF, CNRS, Inst Neel, 25 Rue Martyrs, F-38042 Grenoble, France.
[Berge, L.; Chapellier, M.; Dumoulin, L.; Giuliani, A.; Le-Sueur, H.; Marnieros, S.; Olivieri, E.; Piro, M. -C.; Poda, D.] Univ Paris Saclay, CNRS, IN2P3, CSNSM,Univ Paris Sud, F-91405 Orsay, France.
[Bluemer, J.; Broniatowski, A.; Foerster, N.; Heuermann, G.; Kefelian, C.; Scorza, S.] Karlsruher Inst Technol, Inst Expt Kernphys, Gaedestr 1, D-76128 Karlsruhe, Germany.
[Jin, Y.] CNRS, Lab Photon & Nanostruct, Route Nozay, F-91460 Marcoussis, France.
[Kleifges, M.; Tcherniakhovski, D.; Weber, M.] Karlsruher Inst Technol, Inst Prozessdatenverarbeitung & Elekt, Postfach 3640, D-76021 Karlsruhe, Germany.
[Kraus, H.] Univ Oxford, Dept Phys, Keble Rd, Oxford OX1 3RH, England.
[Kudryavtsev, V. A.] Univ Sheffield, Dept Phys & Astron, Hicks Bldg,Hounsfield Rd, Sheffield S3 7RH, S Yorkshire, England.
[Pari, P.] CEA Saclay, DSM, IRAMIS, F-91191 Gif Sur Yvette, France.
[Rozov, S.; Yakushev, E.] Lab Nucl Problems, JINR, Joliot Curie 6, Dubna 141980, Moscow Region, Russia.
[Arnaud, Q.] Queens Univ, Kingston, ON, Canada.
[Piro, M. -C.] Rensselaer Polytech Inst, Troy, NY USA.
[Schmidt, B.] Lawrence Berkeley Natl Lab, Berkeley, CA USA.
RP Hehn, L (reprint author), Karlsruhe Inst Technol, Inst Kernphys, Postfach 3640, D-76021 Karlsruhe, Germany.
EM lukas.hehn@kit.edu
OI Kudryavtsev, Vitaly/0000-0002-7018-5827
FU German ministry of science and education (BMBF Verbundforschung)
[05A14VKA]; Helmholtz Alliance for Astroparticle Physics (HAP); French
Agence Nationale pour la Recherche (ANR); LabEx Lyon Institute of
Origins of the Universite de Lyon within the program "Investissements
d'Avenir" [ANR-10-LABX-0066, ANR-11-IDEX-00007]; P2IO LabEx in the
framework "Investissements d'Avenir" [ANR-10-LABX-0038,
ANR-11-IDEX-0003-01]; Science and Technology Facilities Council (UK);
Russian Foundation for Basic Research [15-02-03561]
FX The help of the technical staff of the Laboratoire Souterrain de Modane
and the participant laboratories is gratefully acknowledged. EDELWEISS
is supported in part by the German ministry of science and education
(BMBF Verbundforschung ATP Proj.-Nr. 05A14VKA), by the Helmholtz
Alliance for Astroparticle Physics (HAP), by the French Agence Nationale
pour la Recherche (ANR) and the LabEx Lyon Institute of Origins
(ANR-10-LABX-0066) of the Universite de Lyon within the program
"Investissements d'Avenir" (ANR-11-IDEX-00007), by the P2IO LabEx
(ANR-10-LABX-0038) in the framework "Investissements d'Avenir"
(ANR-11-IDEX-0003-01) managed by the ANR (France), by Science and
Technology Facilities Council (UK), and the Russian Foundation for Basic
Research (Grant No. 15-02-03561).
NR 32
TC 0
Z9 0
U1 1
U2 1
PU SPRINGER
PI NEW YORK
PA 233 SPRING ST, NEW YORK, NY 10013 USA
SN 1434-6044
EI 1434-6052
J9 EUR PHYS J C
JI Eur. Phys. J. C
PD OCT 6
PY 2016
VL 76
IS 10
AR 548
DI 10.1140/epjc/s10052-016-4388-y
PG 10
WC Physics, Particles & Fields
SC Physics
GA DY6PJ
UT WOS:000385249500005
ER
PT J
AU Xue, ZH
Hennelly, S
Doyle, B
Gulati, AA
Novikova, IV
Sanbonmatsu, KY
Boyer, LA
AF Xue, Zhihong
Hennelly, Scott
Doyle, Boryana
Gulati, Arune A.
Novikova, Irina V.
Sanbonmatsu, Karissa Y.
Boyer, Laurie A.
TI A G-Rich Motif in the lncRNA Braveheart Interacts with a Zinc-Finger
Transcription Factor to Specify the Cardiovascular Lineage
SO MOLECULAR CELL
LA English
DT Article
ID LONG NONCODING RNAS; ACID-BINDING-PROTEIN; COMPARATIVE
SEQUENCE-ANALYSIS; SECONDARY STRUCTURE; G-QUADRUPLEXES; RIBOSOMAL-RNA;
NUCLEOTIDE-SEQUENCES; MYOTONIC-DYSTROPHY; LIVING CELLS; XIST RNA
AB Long non-coding RNAs (lncRNAs) are an emerging class of transcripts that can modulate gene expression; however, their mechanisms of action remain poorly understood. Here, we experimentally determine the secondary structure of Braveheart (Bvht) using chemical probing methods and show that this similar to 590 nt transcript has a modular fold. Using CRISPR/Cas9-mediated editing of mouse embryonic stem cells, we find that deletion of 11 nt in a 5' asymmetric G-rich internal loop (AGIL) of Bvht (bvht(dAGIL)) dramatically impairs cardiomyocyte differentiation. We demonstrate a specific interaction between AGIL and cellular nucleic acid binding protein (CNBP/ZNF9), a zinc-finger protein known to bind single-stranded G-rich sequences. We further show that CNBP deletion partially rescues the bvht(dAGIL) mutant phenotype by restoring differentiation capacity. Together, our work shows that Bvht functions with CNBP through a well-defined RNA motif to regulate cardiovascular lineage commitment, opening the door for exploring broader roles of RNA structure in development and disease.
C1 [Xue, Zhihong; Gulati, Arune A.; Boyer, Laurie A.] MIT, Dept Biol, 77 Massachusetts Ave, Cambridge, MA 02139 USA.
[Hennelly, Scott; Novikova, Irina V.; Sanbonmatsu, Karissa Y.] Los Alamos Natl Lab, Theoret Biol & Biophys Grp, Los Alamos, NM 87545 USA.
[Hennelly, Scott; Sanbonmatsu, Karissa Y.] New Mexico Consortium, Los Alamos, NM 87544 USA.
[Doyle, Boryana] MIT, Undergrad Res Opportun Program, 77 Massachusetts Ave, Cambridge, MA 02139 USA.
[Doyle, Boryana] MIT, Dept Phys, Cambridge, MA 02139 USA.
[Novikova, Irina V.] Pacific Northwest Natl Lab, Environm Mol Sci Lab, Richmond, WA 99354 USA.
[Boyer, Laurie A.] MIT, Dept Biol Engn, 77 Massachusetts Ave, Cambridge, MA 02139 USA.
RP Boyer, LA (reprint author), MIT, Dept Biol, 77 Massachusetts Ave, Cambridge, MA 02139 USA.; Boyer, LA (reprint author), MIT, Dept Biol Engn, 77 Massachusetts Ave, Cambridge, MA 02139 USA.
EM lboyer@mit.edu
FU LANL-LDRD; Sarnoff Cardiovascular Research Foundation; Koch Institute
[P30CA014051]; NHLBI [U01HL098179]
FX We thank members of the L.A.B. lab, David Bartel, Igor Ulitski, and Matt
Taliaferro for insightful discussions and for critical evaluation of the
manuscript. We also thank Chikdu Shivalila for technical support in
CRIPSR/Cas9 experiments, Lionel Lam for help scanning the protein
microarray, and the flow cytometry core for technical support. K.Y.S.,
S.H., and I.V.N. were supported by LANL-LDRD. A.A.G. was supported by
the Sarnoff Cardiovascular Research Foundation. This work was also
supported in part by the Koch Institute Core grant (P30CA014051) and the
NHLBI Bench to Bassinet Program (U01HL098179) to L.A.B.
NR 79
TC 6
Z9 6
U1 11
U2 11
PU CELL PRESS
PI CAMBRIDGE
PA 600 TECHNOLOGY SQUARE, 5TH FLOOR, CAMBRIDGE, MA 02139 USA
SN 1097-2765
EI 1097-4164
J9 MOL CELL
JI Mol. Cell
PD OCT 6
PY 2016
VL 64
IS 1
BP 37
EP 50
DI 10.1016/j.molcel.2016.08.010
PG 14
WC Biochemistry & Molecular Biology; Cell Biology
SC Biochemistry & Molecular Biology; Cell Biology
GA EE3RO
UT WOS:000389514900008
PM 27618485
ER
PT J
AU Chatterjee, S
Kapoor, A
Akiyama, JA
Auer, DR
Lee, D
Gabriel, S
Berrios, C
Pennacchio, LA
Chakravarti, A
AF Chatterjee, Sumantra
Kapoor, Ashish
Akiyama, Jennifer A.
Auer, Dallas R.
Lee, Dongwon
Gabriel, Stacey
Berrios, Courtney
Pennacchio, Len A.
Chakravarti, Aravinda
TI Enhancer Variants Synergistically Drive Dysfunction of a Gene Regulatory
Network In Hirschsprung Disease
SO CELL
LA English
DT Article
ID ENTERIC NERVOUS-SYSTEM; BETA-GLOBIN GENE; HUMAN GENOME; COMPLEX
DISEASES; RET; COMMON; MICE; EXPRESSION; DNA; DATABASE
AB Common sequence variants in cis-regulatory elements (CREs) are suspected etiological causes of complex disorders. We previously identified an intronic enhancer variant in the RET gene disrupting SOX10 binding and increasing Hirschsprung disease (HSCR) risk 4-fold. We now show that two other functionally independent CRE variants, one binding Gata2 and the other binding Rarb, also reduce Ret expression and increase risk 2- and 1.7-fold. By studying human and mouse fetal gut tissues and cell lines, we demonstrate that reduced RET expression propagates throughout its gene regulatory network, exerting effects on both its positive and negative feedback components. We also provide evidence that the presence of a combination of CRE variants synergistically reduces RET expression and its effects throughout the GRN. These studies show how the effects of functionally independent non-coding variants in a coordinated gene regulatory network amplify their individually small effects, providing a model for complex disorders.
C1 [Chatterjee, Sumantra; Kapoor, Ashish; Auer, Dallas R.; Lee, Dongwon; Berrios, Courtney; Chakravarti, Aravinda] Johns Hopkins Univ, Sch Med, McKusick Nathans Inst Genet Med, Ctr Complex Dis Genom, Baltimore, MD 21205 USA.
[Akiyama, Jennifer A.; Pennacchio, Len A.] Lawrence Berkeley Natl Lab, Genom Div, MS 84-171, Berkeley, CA 94720 USA.
[Gabriel, Stacey] Broad Inst, Cambridge, MA 02142 USA.
[Pennacchio, Len A.] US DOE, Joint Genome Inst, Walnut Creek, CA 94598 USA.
RP Chakravarti, A (reprint author), Johns Hopkins Univ, Sch Med, McKusick Nathans Inst Genet Med, Ctr Complex Dis Genom, Baltimore, MD 21205 USA.
EM aravinda@jhmi.edu
FU NIDCR FaceBase grant [U01DE020060]; NHGRI [R01HG003988, U54HG006997];
Department of Energy [DE-AC02-05CH11231]; Joint MRC/Wellcome Trust Human
Developmental Biology Resource [099175/Z/12/Z]; NIH MERIT Award
[HD28088]
FX We wish to thank our patients and their families, referring physicians,
and genetic counselors for participating in the human genetic studies.
We gratefully acknowledge the assistance of Dr. David Ginty (Harvard
Medical School) for providing Ret mutant mice, Dr. William J. Pavan
(NHGRI, NIH) and Dr. Michael Wegner (Institut fur Biochemie,
Friedrich-Alexander-Universitat) for providing Sox10 mutant mice, and
Dr. Edward Rubin (Lawrence Berkeley National Laboratory) for helpful
discussions. L.A.P. was supported by NIDCR FaceBase grant U01DE020060
and by NHGRI grants R01HG003988 and U54HG006997. The research was
conducted at the E.O. Lawrence Berkeley National Laboratory and
performed under Department of Energy Contract DE-AC02-05CH11231. The
human embryonic and fetal material was provided by the Joint
MRC/Wellcome Trust Human Developmental Biology Resource (www.hdbr.org),
grant number 099175/Z/12/Z. These studies were supported by an NIH MERIT
Award HD28088 to A.C.
NR 54
TC 3
Z9 3
U1 5
U2 5
PU CELL PRESS
PI CAMBRIDGE
PA 600 TECHNOLOGY SQUARE, 5TH FLOOR, CAMBRIDGE, MA 02139 USA
SN 0092-8674
EI 1097-4172
J9 CELL
JI Cell
PD OCT 6
PY 2016
VL 167
IS 2
BP 355
EP +
DI 10.1016/j.cell.2016.09.005
PG 24
WC Biochemistry & Molecular Biology; Cell Biology
SC Biochemistry & Molecular Biology; Cell Biology
GA EA1HM
UT WOS:000386343100013
PM 27693352
ER
PT J
AU Price, MN
Wetmore, KM
Deutschbauer, AM
Arkin, AP
AF Price, Morgan N.
Wetmore, Kelly M.
Deutschbauer, Adam M.
Arkin, Adam P.
TI A Comparison of the Costs and Benefits of Bacterial Gene Expression
SO PLOS ONE
LA English
DT Article
ID ESCHERICHIA-COLI K-12; IN-VIVO; FLUX ANALYSIS; GROWTH; EVOLUTION; YEAST;
POPULATIONS; GLUTATHIONE; METABOLISM; MECHANISMS
AB To study how a bacterium allocates its resources, we compared the costs and benefits of most (86%) of the proteins in Escherichia coli K-12 during growth in minimal glucose medium. The cost or investment in each protein was estimated from ribosomal profiling data, and the benefit of each protein was measured by assaying a library of transposon mutants. We found that proteins that are important for fitness are usually highly expressed, and 95% of these proteins are expressed at above 13 parts per million (ppm). Conversely, proteins that do not measurably benefit the host (with a benefit of less than 5% per generation) tend to be weakly expressed, with a median expression of 13 ppm. In aggregate, genes with no detectable benefit account for 31% of protein production, or about 22% if we correct for genetic redundancy. Although some of the apparently unnecessary expression could have subtle benefits in minimal glucose medium, the majority of the burden is due to genes that are important in other conditions. We propose that at least 13% of the cell's protein is "on standby" in case conditions change.
C1 [Price, Morgan N.; Wetmore, Kelly M.; Deutschbauer, Adam M.; Arkin, Adam P.] Lawrence Berkeley Natl Lab, Environm Genom & Syst Biol, Berkeley, CA 94720 USA.
RP Price, MN (reprint author), Lawrence Berkeley Natl Lab, Environm Genom & Syst Biol, Berkeley, CA 94720 USA.
EM morgannprice@yahoo.com; aparkin@lbl.gov
OI Arkin, Adam/0000-0002-4999-2931; Price, Morgan/0000-0002-4251-0362
FU U.S. Department of Energy, Office of Science, Office of Biological &
Environmental Research [DE-AC02-05CH11231]
FX This material by ENIGMA Ecosystems and Networks Integrated with Genes
and Molecular Assemblies (http://enigma.lbl.gov), a Scientific Focus
Area Program at Lawrence Berkeley National Laboratory, is based upon
work supported by the U.S. Department of Energy, Office of Science,
Office of Biological & Environmental Research under contract number
DE-AC02-05CH11231. The funders had no role in study design, data
collection and analysis, decision to publish, or preparation of the
manuscript.
NR 53
TC 0
Z9 0
U1 9
U2 9
PU PUBLIC LIBRARY SCIENCE
PI SAN FRANCISCO
PA 1160 BATTERY STREET, STE 100, SAN FRANCISCO, CA 94111 USA
SN 1932-6203
J9 PLOS ONE
JI PLoS One
PD OCT 6
PY 2016
VL 11
IS 10
AR e0164314
DI 10.1371/journal.pone.0164314
PG 22
WC Multidisciplinary Sciences
SC Science & Technology - Other Topics
GA DZ2UR
UT WOS:000385697600116
PM 27711251
ER
PT J
AU Dobosz-Bartoszek, M
Pinkerton, MH
Otwinowski, Z
Chakravarthy, S
Soll, D
Copeland, PR
Simonovic, M
AF Dobosz-Bartoszek, Malgorzata
Pinkerton, Mark H.
Otwinowski, Zbyszek
Chakravarthy, Srinivas
Soll, Dieter
Copeland, Paul R.
Simonovic, Miljan
TI Crystal structures of the human elongation factor eEFSec suggest a
non-canonical mechanism for selenocysteine incorporation
SO NATURE COMMUNICATIONS
LA English
DT Article
ID FACTOR-EF-TU; X-RAY STRUCTURES; ESCHERICHIA-COLI; TRANSFER-RNA; FACTOR
SELB; TERNARY COMPLEX; GLUTATHIONE-PEROXIDASE; CONFORMATIONAL-CHANGES;
INSERTION-SEQUENCE; TRANSLATION FACTOR
AB Selenocysteine is the only proteinogenic amino acid encoded by a recoded in-frame UGA codon that does not operate as the canonical opal stop codon. A specialized translation elongation factor, eEFSec in eukaryotes and SelB in prokaryotes, promotes selenocysteine incorporation into selenoproteins by a still poorly understood mechanism. Our structural and biochemical results reveal that four domains of human eEFSec fold into a chalice-like structure that has similar binding affinities for GDP, GTP and other guanine nucleotides. Surprisingly, unlike in eEF1A and EF-Tu, the guanine nucleotide exchange does not cause a major conformational change in domain 1 of eEFSec, but instead induces a swing of domain 4. We propose that eEFSec employs a non-canonical mechanism involving the distinct C-terminal domain 4 for the release of the selenocysteinyl-tRNA during decoding on the ribosome.
C1 [Dobosz-Bartoszek, Malgorzata; Simonovic, Miljan] Univ Illinois, Dept Biochem & Mol Genet, Chicago, IL 60607 USA.
[Pinkerton, Mark H.; Copeland, Paul R.] Rutgers Robert Wood Johnson Med Sch, Dept Biochem & Mol Biol, Piscataway, NJ 08854 USA.
[Otwinowski, Zbyszek] Univ Texas Southwestern Med Ctr Dallas, Dept Biochem, Dallas, TX 75390 USA.
[Chakravarthy, Srinivas] IIT, Biophys Collaborat Access Team, Sect 18ID, Adv Photon Source, Chicago, IL 60439 USA.
[Soll, Dieter] Yale Univ, Dept Mol Biophys & Biochem, POB 6666, New Haven, CT 06520 USA.
[Soll, Dieter] Yale Univ, Dept Chem, 225 Prospect St, New Haven, CT 06520 USA.
RP Simonovic, M (reprint author), Univ Illinois, Dept Biochem & Mol Genet, Chicago, IL 60607 USA.
EM msimon5@uic.edu
RI ID, BioCAT/D-2459-2012
FU University of Illinois at Chicago; American Cancer Society, Illinois
Division [225752]; National Institute of General Medical Sciences
[GM097042, GM070773, GM22854, 1S10D018090-01]; DOE Office of Science
[DE-AC02-06CH11357]; Michigan Technology Tri-Corridor [085P1000817];
National Institute of General Medical Sciences of the National
Institutes of Health [P41 GM103622]
FX We thank the staff of LS-CAT (21-ID) and SBC-CAT (19-ID) beamlines at
the Advanced Photon Source (APS) of the Argonne National Laboratory
(ANL) and organizers of the 7th Annual CCP4 USA Crystallography School
for their help during X-ray data collection and processing, the staff at
the Advanced Protein Characterization Facility (SBC-CAT, APS) for access
to Mosquito crystallization robots and the staff of BioCAT (18-ID)
beamline for help during SAXS data collection. We are grateful to Yury
Polikanov for comments, suggestions and critical reading of the
manuscript. The initial part of the study was supported by the
University of Illinois at Chicago startup fund and a grant from the
American Cancer Society, Illinois Division (225752 to M.S.). The
subsequent studies were supported by grants from the National Institute
of General Medical Sciences (GM097042 to M.S., GM070773 to P.R.C. and
GM22854 to D.S.). This research used resources of the APS, a U.S.
Department of Energy (DOE) Office of Science User Facility operated for
the DOE Office of Science by ANL under contract no. DE-AC02-06CH11357.
Use of the LS-CAT Sector 21 was supported by the Michigan Economic
Development Corporation and the Michigan Technology Tri-Corridor (grant
085P1000817). BioCAT is supported by grant from the National Institute
of General Medical Sciences of the National Institutes of Health (P41
GM103622). Use of the Pilatus 3 1M detector was provided by grant
1S10D018090-01 from the National Institute of General Medical Sciences.
NR 68
TC 1
Z9 1
U1 5
U2 5
PU NATURE PUBLISHING GROUP
PI LONDON
PA MACMILLAN BUILDING, 4 CRINAN ST, LONDON N1 9XW, ENGLAND
SN 2041-1723
J9 NAT COMMUN
JI Nat. Commun.
PD OCT 6
PY 2016
VL 7
AR 12941
DI 10.1038/ncomms12941
PG 11
WC Multidisciplinary Sciences
SC Science & Technology - Other Topics
GA DZ0TW
UT WOS:000385553600002
PM 27708257
ER
PT J
AU Ozaki, T
Wu, LJ
Zhang, C
Jaroszynski, J
Si, WD
Zhou, J
Zhu, YM
Li, Q
AF Ozaki, Toshinori
Wu, Lijun
Zhang, Cheng
Jaroszynski, Jan
Si, Weidong
Zhou, Juan
Zhu, Yimei
Li, Qiang
TI A route for a strong increase of critical current in nanostrained
iron-based superconductors
SO NATURE COMMUNICATIONS
LA English
DT Article
ID CRITICAL-CURRENT-DENSITY; BA(FE1-XCOX)(2)AS-2 THIN-FILMS; FINAL
OPTIMIZATION STRAIN; NB-TI SUPERCONDUCTOR; QUANTITATIVE DESCRIPTION;
CRITICAL-TEMPERATURE; ELECTRON-MICROSCOPY; IRRADIATION DEFECTS; PINNING
MECHANISM; PHASE-DIAGRAM
AB The critical temperature T-c and the critical current density J(c) determine the limits to large-scale superconductor applications. Superconductivity emerges at T-c. The practical current-carrying capability, measured by J(c), is the ability of defects in superconductors to pin the magnetic vortices, and that may reduce T-c. Simultaneous increase of T-c and J(c) in superconductors is desirable but very difficult to realize. Here we demonstrate a route to raise both T-c and J(c) together in iron-based superconductors. By using low-energy proton irradiation, we create cascade defects in FeSe0.5Te0.5 films. T-c is enhanced due to the nanoscale compressive strain and proximity effect, whereas J(c) is doubled under zero field at 4.2 K through strong vortex pinning by the cascade defects and surrounding nanoscale strain. At 12 K and above 15 T, one order of magnitude of J(c) enhancement is achieved in both parallel and perpendicular magnetic fields to the film surface.
C1 [Ozaki, Toshinori; Wu, Lijun; Zhang, Cheng; Si, Weidong; Zhou, Juan; Zhu, Yimei; Li, Qiang] Brookhaven Natl Lab, Condensed Matter Phys & Mat Sci Dept, Upton, NY 11973 USA.
[Ozaki, Toshinori] Kwansei Gakuin Univ, Dept Nanotechnol Sustainable Energy, 2-1 Gakuen, Sanda, Hyogo 6691337, Japan.
[Jaroszynski, Jan] Florida State Univ, Natl High Magnet Field Lab, 1800 E Paul Dirac Dr, Tallahassee, FL 32310 USA.
RP Ozaki, T; Li, Q (reprint author), Brookhaven Natl Lab, Condensed Matter Phys & Mat Sci Dept, Upton, NY 11973 USA.
EM tozaki@kwansei.ac.jp; qiangli@bnl.gov
RI Zhang, Cheng/R-6593-2016
OI Zhang, Cheng/0000-0001-6531-4703
FU US Department of Energy, Office of Basic Energy Science, Materials
Sciences and Engineering Division [DE-SC00112704]; National Science
Foundation [DMR-1157490]; State of Florida; US Department of Energy
FX This work was supported by the US Department of Energy, Office of Basic
Energy Science, Materials Sciences and Engineering Division, under
contract number DE-SC00112704. High-field Jc measurement was
performed at the National High Magnetic Field Laboratory, which is
supported by National Science Foundation Cooperative Agreement Number
DMR-1157490, the State of Florida and the US Department of Energy.
NR 66
TC 1
Z9 1
U1 25
U2 25
PU NATURE PUBLISHING GROUP
PI LONDON
PA MACMILLAN BUILDING, 4 CRINAN ST, LONDON N1 9XW, ENGLAND
SN 2041-1723
J9 NAT COMMUN
JI Nat. Commun.
PD OCT 6
PY 2016
VL 7
AR 13036
DI 10.1038/ncomms13036
PG 9
WC Multidisciplinary Sciences
SC Science & Technology - Other Topics
GA DZ0UX
UT WOS:000385556300001
PM 27708268
ER
PT J
AU Xiang, YZ
Kruse, N
AF Xiang, Yizhi
Kruse, Norbert
TI Tuning the catalytic CO hydrogenation to straight- and long-chain
aldehydes/alcohols and olefins/paraffins
SO NATURE COMMUNICATIONS
LA English
DT Article
ID FISCHER-TROPSCH SYNTHESIS; CARBON-MONOXIDE; HIGHER ALCOHOLS; IRON
CATALYSTS; OXYGENATE SELECTIVITY; COBALT CARBIDE; NANOPARTICLES;
STABILITY; PROMOTER; OLEFINS
AB The catalytic CO hydrogenation is one of the most versatile large-scale chemical syntheses leading to variable chemical feedstock. While traditionally mainly methanol and long-chain hydrocarbons are produced by CO hydrogenation, here we show that the same reaction can be tuned to produce long-chain n-aldehydes, 1-alcohols and olefins, as well as n-paraffins over potassium-promoted CoMn catalysts. The sum selectivity of aldehydes and alcohols is usually >50 wt% whereof up to similar to 97% can be n-aldehydes. While the product slate contains similar to 60% n-aldehydes at p(H2)/p(CO) = 0.5, a 65/35% slate of paraffins/alcohols is obtained at a ratio of 9. A linear Anderson-Schulz-Flory behaviour, independent of the p(H2)/p(CO) ratio, is found for the sum of C4+ products. We advocate a synergistic interaction between a Mn5O8 oxide and a bulk Co2C phase, promoted by the presence of potassium, to be responsible for the unique product spectra in our studies.
C1 [Xiang, Yizhi; Kruse, Norbert] Washington State Univ, Voiland Sch Chem Engn & Bioengn, Pullman, WA 99164 USA.
[Kruse, Norbert] Pacific Northwest Natl Lab, Inst Integrated Catalysis, Richland, WA 99332 USA.
RP Kruse, N (reprint author), Washington State Univ, Voiland Sch Chem Engn & Bioengn, Pullman, WA 99164 USA.; Kruse, N (reprint author), Pacific Northwest Natl Lab, Inst Integrated Catalysis, Richland, WA 99332 USA.
EM norbert.kruse@wsu.edu
FU National Science Foundation [CBET-1438227]
FX The project has been gratefully supported by National Science Foundation
under contract no. CBET-1438227. We sincerely thank Professor Xiaonian
Li (Industrial Catalysis Institute of Zhejiang University of Technology)
for assisting with HRTEM measurements and Dr Libor Kovarik (Pacific
Northwest National Laboratory) for helping with HAADF-TEM measurements.
NR 35
TC 4
Z9 4
U1 45
U2 45
PU NATURE PUBLISHING GROUP
PI LONDON
PA MACMILLAN BUILDING, 4 CRINAN ST, LONDON N1 9XW, ENGLAND
SN 2041-1723
J9 NAT COMMUN
JI Nat. Commun.
PD OCT 6
PY 2016
VL 7
AR 13058
DI 10.1038/ncomms13058
PG 6
WC Multidisciplinary Sciences
SC Science & Technology - Other Topics
GA DZ0VB
UT WOS:000385556700001
PM 27708269
ER
PT J
AU Roy, S
Kolodrubetz, M
Moore, JE
Grushin, AG
AF Roy, Sthitadhi
Kolodrubetz, Michael
Moore, Joel E.
Grushin, Adolfo G.
TI Chern numbers and chiral anomalies in Weyl butterflies
SO PHYSICAL REVIEW B
LA English
DT Article
ID DIRAC SEMIMETAL CD3AS2; TOPOLOGICAL INSULATORS; FERMI ARCS; NEGATIVE
MAGNETORESISTANCE; MAGNETIC-FIELD; PHASE; DISCOVERY; ATOMS; TAAS;
DIMENSIONS
AB The Hofstadter butterfly of lattice electrons in a strong magnetic field is a cornerstone of condensed matter physics, exploring the competition between periodicities imposed by the lattice and the field. Here, we introduce and characterize the Weyl butterfly, which emerges when a large magnetic field is applied to a three-dimensional Weyl semimetal. Using an experimentally motivated lattice model for cold-atomic systems, we solve this problem numerically. We find that Weyl nodes reemerge at commensurate fluxes and propose using wave-packet dynamics to reveal their chirality and location. Moreover, we show that the chiral anomaly-a hallmark of the topological Weyl semimetal-does not remain proportional to the magnetic field at large fields, but rather inherits a fractal structure of linear regimes as a function of the external field. The slope of each linear regime is determined by the difference of two Chern numbers in the gaps of the Weyl butterfly and can be measured experimentally in time of flight.
C1 [Roy, Sthitadhi] Max Planck Inst Phys Komplexer Syst, Nothnitzer Str 38, D-01187 Dresden, Germany.
[Kolodrubetz, Michael; Moore, Joel E.] Lawrence Berkeley Natl Lab, Div Mat Sci, Berkeley, CA 94720 USA.
[Kolodrubetz, Michael; Moore, Joel E.; Grushin, Adolfo G.] Univ Calif Berkeley, Dept Phys, Berkeley, CA 94720 USA.
RP Roy, S (reprint author), Max Planck Inst Phys Komplexer Syst, Nothnitzer Str 38, D-01187 Dresden, Germany.
RI Moore, Joel/O-4959-2016
OI Moore, Joel/0000-0002-4294-5761
FU European Commission under the Marie Curie Programme; Laboratory Directed
Research and Development (LDRD) from Berkeley Lab by Office of Science,
of the U.S. Department of Energy [DEAC02-05CH11231]; Simons Investigator
grant
FX A.G.G. acknowledges financial support from the European Commission under
the Marie Curie Programme. We thank C. Kennedy for useful insights on
the experimental feasibility of this proposal. M.K. and J.E.M. were
supported by Laboratory Directed Research and Development (LDRD) funding
from Berkeley Lab, provided by the Director, Office of Science, of the
U.S. Department of Energy under Contract No. DEAC02-05CH11231, and
J.E.M. acknowledges support from a Simons Investigator grant.
NR 79
TC 0
Z9 0
U1 10
U2 10
PU AMER PHYSICAL SOC
PI COLLEGE PK
PA ONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA
SN 2469-9950
EI 2469-9969
J9 PHYS REV B
JI Phys. Rev. B
PD OCT 6
PY 2016
VL 94
IS 16
AR 161107
DI 10.1103/PhysRevB.94.161107
PG 7
WC Physics, Condensed Matter
SC Physics
GA DY6NE
UT WOS:000385243200002
ER
PT J
AU Linder, EV
AF Linder, Eric V.
TI Doubling strong lensing as a cosmological probe
SO PHYSICAL REVIEW D
LA English
DT Article
ID TIME-DELAY COSMOGRAPHY; EQUATION-OF-STATE; HUBBLE CONSTANT; STRONG
LENSES; PARAMETERS; PRECISION; SYSTEMS
AB Strong gravitational lensing provides a geometric probe of cosmology in a unique manner through distance ratios involving the source and lens. This is well-known for the time delay distance derived from measured delays between lightcurves of the images of variable sources such as quasars. Recently, double source plane lens systems involving two constant sources lensed by the same foreground lens have been proposed as another probe, involving a different ratio of distances measured from the image positions and fairly insensitive to the lens modeling. Here we demonstrate that these two different sets of strong lensing distance ratios have strong complementarity in cosmological leverage. Unlike other probes, the double source distance ratio is actually more sensitive to the dark energy equation of state parameters w(0) and w(a) than to the matter density Omega(m), for low redshift lenses. Adding double source distance ratio measurements can improve the dark energy figure of merit by 40% for a sample of fewer than 100 low redshift systems, or even better for the optimal redshift distribution we derive.
C1 [Linder, Eric V.] Univ Calif Berkeley, Berkeley Ctr Cosmol Phys, Berkeley, CA 94720 USA.
[Linder, Eric V.] Univ Calif Berkeley, Berkeley Lab, Berkeley, CA 94720 USA.
RP Linder, EV (reprint author), Univ Calif Berkeley, Berkeley Ctr Cosmol Phys, Berkeley, CA 94720 USA.; Linder, EV (reprint author), Univ Calif Berkeley, Berkeley Lab, Berkeley, CA 94720 USA.
FU U.S. Department of Energy, Office of Science, Office of High Energy
Physics [DE-SC-0007867, DE-AC02-05CH11231]
FX I thank the Institute of Cosmology and Gravitation, University of
Portsmouth for hospitality during the ICG-KASI workshop that inspired
this work, and Tom Collett for informative discussions. This work is
supported in part by the U.S. Department of Energy, Office of Science,
Office of High Energy Physics, under Award No. DE-SC-0007867 and
Contract No. DE-AC02-05CH11231.
NR 36
TC 0
Z9 0
U1 2
U2 2
PU AMER PHYSICAL SOC
PI COLLEGE PK
PA ONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA
SN 2470-0010
EI 2470-0029
J9 PHYS REV D
JI Phys. Rev. D
PD OCT 6
PY 2016
VL 94
IS 8
AR 083510
DI 10.1103/PhysRevD.94.083510
PG 7
WC Astronomy & Astrophysics; Physics, Particles & Fields
SC Astronomy & Astrophysics; Physics
GA DY6OL
UT WOS:000385246500004
ER
PT J
AU Dinh, LN
Sun, TC
McLean, W
AF Dinh, L. N.
Sun, T. C.
McLean, W., II
TI Temperature-Dependent Kinetic Prediction for Reactions Described by
Isothermal Mathematics
SO JOURNAL OF PHYSICAL CHEMISTRY A
LA English
DT Article
ID SOLID-STATE KINETICS; VARYING ACTIVATION-ENERGIES; ISOCONVERSIONAL
METHODS; NONISOTHERMAL KINETICS; RUNAWAY REACTIONS; HAZARDS
AB Most kinetic models are expressed in isothermal mathematics. This may lead unaware scientists either to the misconception that classical isothermal kinetic models cannot be used for any chemical process in an environment with a time-dependent temperature profile or, even worse, to a misuse of them. In reality, classical isothermal models can be employed to make kinetic predictions for reactions in environments with time-dependent temperature profiles, provided that there is a continuity/conservation in the reaction extent at every temperature time step. In this article, fundamental analyses, illustrations, guiding tables, and examples are given to help the interested readers using either conventional isothermal reacted fraction curves or rate equations to make proper kinetic predictions for chemical reactions in environments with temperature profiles that vary, even arbitrarily, with time simply by the requirement of continuity/conservation of reaction extent whenever there is an external temperature change.
C1 [Dinh, L. N.; Sun, T. C.; McLean, W., II] Lawrence Livermore Natl Lab, Livermore, CA 94550 USA.
RP Dinh, LN (reprint author), Lawrence Livermore Natl Lab, Livermore, CA 94550 USA.
EM dinh1@llnl.gov
FU U.S. Department of Energy by Lawrence Livermore National Laboratory
[DE-AC52-07NA27344]
FX This work was performed under the auspices of the U.S. Department of
Energy by Lawrence Livermore National Laboratory under Contract
DE-AC52-07NA27344.
NR 25
TC 0
Z9 0
U1 2
U2 2
PU AMER CHEMICAL SOC
PI WASHINGTON
PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA
SN 1089-5639
J9 J PHYS CHEM A
JI J. Phys. Chem. A
PD OCT 6
PY 2016
VL 120
IS 39
BP 7617
EP 7623
DI 10.1021/acs.jpca.6b08219
PG 7
WC Chemistry, Physical; Physics, Atomic, Molecular & Chemical
SC Chemistry; Physics
GA DY2YZ
UT WOS:000384959300004
PM 27617790
ER
PT J
AU Dantas, JM
Simoes, T
Morgado, L
Caciones, C
Fernandes, AP
Silva, MA
Bruix, M
Pokkuluri, PR
Salgueiro, CA
AF Dantas, Joana M.
Simoes, Telma
Morgado, Leonor
Caciones, Clara
Fernandes, Ana P.
Silva, Marta A.
Bruix, Marta
Pokkuluri, P. Raj
Salgueiro, Carlos A.
TI Unveiling the Structural Basis That Regulates the Energy Transduction
Properties within a Family of Triheme Cytochromes from Geobacter
sulfurreducens
SO JOURNAL OF PHYSICAL CHEMISTRY B
LA English
DT Article
ID AROMATIC RESIDUE F-15; ELECTRON-TRANSFER; REDOX PROPERTIES; C(7);
ELECTRICITY; METABOLISM; PROTEINS; ECOLOGY; MUTANT; PPCA
AB A family of triheme cytochromes from Geobacter sulfurreducens plays an important role in extracellular electron transfer. In addition to their role in electron transfer pathways, two members of this family (PpcA and PpcD) were also found to be able to couple e(-)/H+ transfer through the redox Bohr effect observed in the physiological pH range, a feature not observed for cytochromes PpcB and PpcE. In attempting to understand the molecular control of the redox Bohr effect in this family of cytochromes, which is highly homologous both in amino acid sequence and structures, it was observed that residue 6 is a conserved leucine in PpcA and PpcD, whereas in the other two characterized members (PpcB and PpcE) the equivalent residue is a phenylalanine. To determine the role of this residue located close to the redox Bohr center, we replaced Leu(6) in PpcA with Phe and determined the redox properties of the mutant, as well as its solution structure in the fully reduced state. In contrast with the native form, the mutant PpcAL6F is not able to couple the e(-)/H+ pathway. We carried out the reverse mutation in PpcB and PpcE (i.e., replacing Phe(6) in these two proteins by leucine) and the mutated proteins showed an increased redox Bohr effect. The results clearly establish the role of residue 6 in the control of the redox Bohr effect in this family of cytochromes, a feature that could enable the rational design of G. sulfurreducens strains that carry mutant cytochromes with an optimal redox Bohr effect that would be suitable for various biotechnological applications.
C1 [Dantas, Joana M.; Simoes, Telma; Morgado, Leonor; Caciones, Clara; Fernandes, Ana P.; Silva, Marta A.; Salgueiro, Carlos A.] Univ Nova Lisboa, Fac Ciencias & Tecnol, Dept Quim, UCIBIO Requimte, Campus Caparica, P-2829516 Caparica, Portugal.
[Bruix, Marta] CSIC, Inst Quim Fis Rocasolano, Dept Quim Fis Biol, Madrid 28006, Spain.
[Pokkuluri, P. Raj] Argonne Natl Lab, Biosci Div, 9700 S Cass Ave, Argonne, IL 60439 USA.
[Morgado, Leonor] Univ Basel, Biozentrum, Basel, Switzerland.
RP Salgueiro, CA (reprint author), Univ Nova Lisboa, Fac Ciencias & Tecnol, Dept Quim, UCIBIO Requimte, Campus Caparica, P-2829516 Caparica, Portugal.
EM csalgueiro@fct.unl.pt
RI Bruix, Marta/H-4161-2011; Dantas, Joana/B-8275-2017
OI Bruix, Marta/0000-0002-0096-3558; Dantas, Joana/0000-0002-4852-7608
FU Fundacao para a Ciencia e a Tecnologia, Portugal [UID/Multi/04378/2013];
Fundacao para a Ciencia e a Tecnologia [RECl/BBB-BQB/0230/2012];
Division of Chemical Sciences, Geosciences, and Biosciences, Office of
Basic Energy Sciences of the U.S. Department of Energy program
[DE-AC02-06CH11357]; [PTDC/BBB-BQB/3554/2014]; [SFRH/BD/89701/2012];
[SFRH/BD/86439/2012]; [SFRH/BD/61952/2009]
FX D.L. Turner is acknowledged for providing the software programs used to
calculate the thermodynamic parameters and the solution structure. This
work was supported by the following project grants:
PTDC/BBB-BQB/3554/2014 (to C.A.S.); SFRH/BD/89701/2012,
SFRH/BD/86439/2012, and SFRH/BD/61952/2009 (to J.M.D., A.P.F., and
M.A.S., respectively), and UID/Multi/04378/2013 from Fundacao para a
Ciencia e a Tecnologia, Portugal. The NMR spectrometers are part of The
National NMR Facility, supported by Fundacao para a Ciencia e a
Tecnologia (RECl/BBB-BQB/0230/2012). P.R.P. is partially supported by
the Division of Chemical Sciences, Geosciences, and Biosciences, Office
of Basic Energy Sciences of the U.S. Department of Energy program under
contract no. DE-AC02-06CH11357.
NR 27
TC 0
Z9 0
U1 6
U2 6
PU AMER CHEMICAL SOC
PI WASHINGTON
PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA
SN 1520-6106
J9 J PHYS CHEM B
JI J. Phys. Chem. B
PD OCT 6
PY 2016
VL 120
IS 39
BP 10221
EP 10233
DI 10.1021/acs.jpcb.6b07059
PG 13
WC Chemistry, Physical
SC Chemistry
GA DY2YY
UT WOS:000384959200006
PM 27603556
ER
PT J
AU Krishnan, S
Sharma, V
Singh, P
Ramprasad, R
AF Krishnan, Sridevi
Sharma, Vinit
Singh, Prabhakar
Ramprasad, Rampi
TI Dopants in Lanthanum Manganite: Insights from First-Principles Chemical
Space Exploration
SO JOURNAL OF PHYSICAL CHEMISTRY C
LA English
DT Article
ID COMPUTATIONAL MATERIALS DESIGN; DENSITY-FUNCTIONAL THEORY; TOTAL-ENERGY
CALCULATIONS; OXIDE FUEL-CELLS; WAVE BASIS-SET; DOPED LAMNO3;
ELECTRONIC-STRUCTURE; POLYMER DIELECTRICS; QUANTUM-MECHANICS; PEROVSKITE
OXIDES
AB The dopant chemical space in LaMnO3 (LMO) is systematically explored using first-principles computations. We study a range of cationic dopants including alkali, alkaline earth metals, 3d, 4d, and 5d transition metal elements without and with an adjacent O vacancy. A linear programming approach is employed to access the energetically favorable decomposition pathway and the corresponding decomposition energy of doped LaMnO3. The decomposition energy is then used to classify the dopants for stability, site preference and tendency of O vacancy formation. We find that La site doping is more favored compared to Mn site doping. We also identify dopants previously not considered, such as K, Rb, Cs, and In, which lead to stable doped LMO and are also excellent O vacancy formers. Employing data mining techniques, we identify the dopant features that are critical to the stability of a doped oxide.
C1 [Krishnan, Sridevi; Sharma, Vinit; Singh, Prabhakar; Ramprasad, Rampi] Univ Connecticut, Mat Sci & Engn, Storrs, CT 06269 USA.
[Krishnan, Sridevi; Sharma, Vinit; Ramprasad, Rampi] Univ Connecticut, Inst Mat Sci, Storrs, CT 06269 USA.
[Singh, Prabhakar] Univ Connecticut, Ctr Clean Energy Engn, Storrs, CT 06269 USA.
[Sharma, Vinit] Oak Ridge Natl Lab, Div Mat Sci & Technol, Oak Ridge, TN 37831 USA.
RP Krishnan, S; Ramprasad, R (reprint author), Univ Connecticut, Mat Sci & Engn, Storrs, CT 06269 USA.; Krishnan, S; Ramprasad, R (reprint author), Univ Connecticut, Inst Mat Sci, Storrs, CT 06269 USA.
EM sridevi.krishnan@uconn.edu; rampi.ramprasad@uconn.edu
FU Office of Fossil Energy, US Department of Energy [DE-FE-0009682]
FX This work is supported, in part, through a grant from the Office of
Fossil Energy, US Department of Energy (DE-FE-0009682). The authors
acknowledge partial computational support through the Extreme Science
and Engineering Discovery Environment (XSEDE). V.S. acknowledges the
XSEDE computational resource allocation number TG-DMR160051.
NR 68
TC 1
Z9 1
U1 12
U2 12
PU AMER CHEMICAL SOC
PI WASHINGTON
PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA
SN 1932-7447
J9 J PHYS CHEM C
JI J. Phys. Chem. C
PD OCT 6
PY 2016
VL 120
IS 39
BP 22126
EP 22133
DI 10.1021/acs.jpcc.6b04524
PG 8
WC Chemistry, Physical; Nanoscience & Nanotechnology; Materials Science,
Multidisciplinary
SC Chemistry; Science & Technology - Other Topics; Materials Science
GA DY2YX
UT WOS:000384959100002
ER
PT J
AU Plakhova, TV
Romanchuk, AY
Yakunin, SN
Dumas, T
Demir, S
Wang, SA
Minasian, SG
Shuh, DK
Tyliszczak, T
Shiryaev, AA
Egorov, AV
Ivanov, VK
Kalmykov, SN
AF Plakhova, Tatiana V.
Romanchuk, Anna Yu.
Yakunin, Sergey N.
Dumas, Thomas
Demir, Selvan
Wang, Shuao
Minasian, Stefan G.
Shuh, David K.
Tyliszczak, Tolek
Shiryaev, Andrey A.
Egorov, Alexander V.
Ivanov, Vladimir K.
Kalmykov, Stepan N.
TI Solubility of Nanocrystalline Cerium Dioxide: Experimental Data and
Thermodynamic Modeling
SO JOURNAL OF PHYSICAL CHEMISTRY C
LA English
DT Article
ID X-RAY-ABSORPTION; STRUCTURE-SENSITIVE PROPERTIES; DENSITY-FUNCTIONAL
THEORY; ADVANCED LIGHT-SOURCE; OXYGEN K-EDGE; OXIDE NANOPARTICLES; CEO2
NANOPARTICLES; REDUCTIVE DISSOLUTION; PHOTOELECTRON-SPECTROSCOPY;
BIOMEDICAL APPLICATIONS
AB Ultrafine 5 nm ceria isotropic nanoparticles were prepared using the rapid chemical precipitation approach from cerium(III) nitrate and ammonium hydroxide aqueous solutions. The as-prepared nanoparticles were shown to contain predominantly Ce(IV) species. The solubility of nanocrystalline CeO2 at several pH values was determined using ICP-MS and radioactive tracer methods. Phase composition of the ceria samples remained unchanged upon partial dissolution, while the shape of the particles changed dramatically, yielding nanorods under neutral pH conditions. According to X-ray absorption spectroscopy investigation of the supernatant, Ce(III) was the main cerium species in solution at pH < 4. Based on the results obtained, a reductive dissolution model was used for data interpretation. According to this model, the solubility product for ceria nanoparticles was determined to be log K-sp = -59.3 +/- 0.3 in 0.01 M NaClO4. Taken together, our results show that the pH dependence of ceria anti- and pro-oxidant activity can be related to the dissolution of CeO2 in aqueous media.
C1 [Plakhova, Tatiana V.; Romanchuk, Anna Yu.; Shiryaev, Andrey A.; Egorov, Alexander V.; Ivanov, Vladimir K.; Kalmykov, Stepan N.] Lomonosov Moscow State Univ, Moscow, Russia.
[Yakunin, Sergey N.; Kalmykov, Stepan N.] Kurchatov Inst, Natl Res Ctr, Moscow, Russia.
[Dumas, Thomas] CEA DEN MAR DRCP, Radiochem & Proc Dept, Nucl Energy Div, BP17171, F-30207 Bagnols Sur Ceze, France.
[Demir, Selvan; Wang, Shuao] Lawrence Berkeley Natl Lab, Div Chem Sci, Berkeley, CA 94720 USA.
[Tyliszczak, Tolek] Lawrence Berkeley Natl Lab, Adv Light Source, Berkeley, CA 94720 USA.
[Demir, Selvan; Wang, Shuao; Minasian, Stefan G.; Shuh, David K.] Univ Calif Berkeley, Dept Chem, Berkeley, CA 94720 USA.
[Shiryaev, Andrey A.] Russian Acad Sci, Frumkin Inst Phys Chem & Electrochem, Moscow, Russia.
[Ivanov, Vladimir K.] Russian Acad Sci, Kurnakov Inst Gen & Inorgan Chem, Moscow, Russia.
[Ivanov, Vladimir K.] Tomsk State Univ, Natl Res, Tomsk, Russia.
RP Kalmykov, SN (reprint author), Lomonosov Moscow State Univ, Moscow, Russia.; Kalmykov, SN (reprint author), Kurchatov Inst, Natl Res Ctr, Moscow, Russia.
EM stepan@radio.chem.msu.ru
RI Ivanov, Vladimir/H-4407-2011; Shiryaev, Andrei/F-7643-2012; dumas,
thomas/B-5950-2016
OI Ivanov, Vladimir/0000-0003-2343-2140; dumas, thomas/0000-0001-6425-6484
FU RFBR [16-31-06000 mol_a_dk, 16-33-00650 mol_a]; HRTEM measurements;
Office of Science, Office of Basic Energy Sciences (BES), Division of
Chemical Sciences, Geosciences, and Biosciences (CSGB) Heavy Element
Chemistry Programme of the U.S. Department of Energy (DOE) at the
Lawrence Berkeley National Laboratory (LBNL) [DE-AC02-05CH11231]; Office
of Science, BES, of the U.S. DOE [DE-AC02-05CH11231]; Office of Science,
BES, CSGB Condensed Phase and Interfacial Molecular Sciences Programme
by the U.S. DOE at LBNL [DE-AC02-05CH11231]
FX The study was funded by RFBR, according to the research projects No.
16-31-06000 mol_a_dk and No. 16-33-00650 mol_a. The authors thank the
M.V. Lomonosov Moscow State University Programme of Development and A.
V. Garshev for partial support of HRTEM measurements. We are also
grateful to the "Nanochemistry and Nanomaterials" user facility of the
Department of Chemistry of MSU for providing the HRTEM and XPS
measurements. SAXS measurements were performed using equipment of CKP
FMI IPCE RAS. S.G.M. and D.K.S. were supported by the Director, Office
of Science, Office of Basic Energy Sciences (BES), Division of Chemical
Sciences, Geosciences, and Biosciences (CSGB) Heavy Element Chemistry
Programme of the U.S. Department of Energy (DOE) at the Lawrence
Berkeley National Laboratory (LBNL), under Contract DE-AC02-05CH11231.
MES Beamline 11.0.2.2 at the ALS was supported by the Director, Office
of Science, BES, CSGB Condensed Phase and Interfacial Molecular Sciences
Programme by the U.S. DOE at LBNL, under Contract DE-AC02-05CH11231. The
ALS and TT were supported by the Director, Office of Science, BES, of
the U.S. DOE, under Contract DE-AC02-05CH11231 at LBNL.
NR 104
TC 2
Z9 2
U1 23
U2 23
PU AMER CHEMICAL SOC
PI WASHINGTON
PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA
SN 1932-7447
J9 J PHYS CHEM C
JI J. Phys. Chem. C
PD OCT 6
PY 2016
VL 120
IS 39
BP 22615
EP 22626
DI 10.1021/acs.jpcc.6b05650
PG 12
WC Chemistry, Physical; Nanoscience & Nanotechnology; Materials Science,
Multidisciplinary
SC Chemistry; Science & Technology - Other Topics; Materials Science
GA DY2YX
UT WOS:000384959100056
ER
PT J
AU Chou, SS
Swartzentruber, BS
Janish, MT
Meyer, KC
Biedermann, LB
Okur, S
Burckel, DB
Carter, CB
Kaehr, B
AF Chou, Stanley S.
Swartzentruber, Brian S.
Janish, Matthew T.
Meyer, Kristin C.
Biedermann, Laura B.
Okur, Serdal
Burckel, D. Bruce
Carter, C. Barry
Kaehr, Bryan
TI Laser Direct Write Synthesis of Lead Halide Perovskites
SO JOURNAL OF PHYSICAL CHEMISTRY LETTERS
LA English
DT Article
ID SOLAR-CELLS; NANOWIRE; LITHOGRAPHY; CATALYSIS; CRYSTALS; GROWTH
AB Lead halide perovskites are increasingly considered for applications beyond photovoltaics, for example, light emission and detection, where an ability to pattern and prototype microscale geometries can facilitate the incorporation of this class of materials into devices. Here we demonstrate laser direct write of lead halide perovskites, a remarkably simple procedure that takes advantage of the inverse dependence between perovskite solubility and temperature by using a laser to induce localized heating of an absorbing substrate. We demonstrate arbitrary pattern formation of crystalline CH3NH3PbBr3 on a range of substrates and fabricate and characterize a microscale photodetector using this approach. This direct write methodology provides a path forward for the prototyping and production of perovskite-based devices.
C1 [Chou, Stanley S.; Biedermann, Laura B.; Burckel, D. Bruce] Sandia Natl Labs, POB 5800, Albuquerque, NM 87185 USA.
[Swartzentruber, Brian S.; Carter, C. Barry] Sandia Natl Labs, Ctr Integrated Nanotechnol, Albuquerque, NM 87545 USA.
[Janish, Matthew T.; Carter, C. Barry] Univ Connecticut, Dept Mat Sci & Engn, Storrs, CT 06269 USA.
[Meyer, Kristin C.; Kaehr, Bryan] Sandia Natl Labs, Adv Mat Lab, Albuquerque, NM 87106 USA.
[Okur, Serdal] Univ New Mexico, Dept Elect & Comp Engn, Albuquerque, NM 87131 USA.
[Kaehr, Bryan] Univ New Mexico, Dept Chem & Biol Engn, Albuquerque, NM 87131 USA.
RP Chou, SS (reprint author), Sandia Natl Labs, POB 5800, Albuquerque, NM 87185 USA.; Kaehr, B (reprint author), Sandia Natl Labs, Adv Mat Lab, Albuquerque, NM 87106 USA.; Kaehr, B (reprint author), Univ New Mexico, Dept Chem & Biol Engn, Albuquerque, NM 87131 USA.
EM schou@sandia.gov; bjkaehr@sandia.gov
RI Okur, Serdal/D-3765-2015
OI Okur, Serdal/0000-0002-0391-3492
FU U.S. Department of Energy, Office of Science, Basic Energy Sciences,
Materials Sciences and Engineering Division; U.S. Department of Energy's
National Nuclear Security Administration [DE AC04-94AL85000]
FX This work was supported by the U.S. Department of Energy, Office of
Science, Basic Energy Sciences, Materials Sciences and Engineering
Division. This work was performed, in part, at the Center for Integrated
Nanotechnologies, a U.S. Department of Energy, Office of Basic Energy
Sciences user facility. Sandia National Laboratories is a multi-mission
laboratory managed and operated by Sandia Corporation, a wholly owned
subsidiary of Lockheed Martin Corporation, for the U.S. Department of
Energy's National Nuclear Security Administration under Contract No. DE
AC04-94AL85000.
NR 28
TC 1
Z9 1
U1 22
U2 22
PU AMER CHEMICAL SOC
PI WASHINGTON
PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA
SN 1948-7185
J9 J PHYS CHEM LETT
JI J. Phys. Chem. Lett.
PD OCT 6
PY 2016
VL 7
IS 19
BP 3736
EP 3741
DI 10.1021/acs.jpclett.6b01557
PG 6
WC Chemistry, Physical; Nanoscience & Nanotechnology; Materials Science,
Multidisciplinary; Physics, Atomic, Molecular & Chemical
SC Chemistry; Science & Technology - Other Topics; Materials Science;
Physics
GA DY3BT
UT WOS:000384966500005
PM 27593712
ER
PT J
AU Sachs, M
Pastor, E
Kafizas, A
Durrant, JR
AF Sachs, Michael
Pastor, Ernest
Kafizas, Andreas
Durrant, James R.
TI Evaluation of Surface State Mediated Charge Recombination in Anatase and
Rutile TiO2
SO JOURNAL OF PHYSICAL CHEMISTRY LETTERS
LA English
DT Article
ID TRANSIENT ABSORPTION-SPECTROSCOPY; SOLAR-CELLS; LOW-COST; FEMTOSECOND;
EFFICIENCY; DYNAMICS; POWDERS; HOLES; PHOTOELECTRODES; PHOTOCATALYSIS
AB In nanostructured thin films, photogenerated charge carriers can access the surface more easily than in dense films and thus react more readily. However, the high surface area of these films has also been associated with enhanced recombination losses via surface states. We herein use transient absorption spectroscopy to compare the ultrafast charge carrier kinetics in dense and nanostructured TiO2 films for its two most widely used polymorphs: anatase and rutile. We find that nanostructuring does not enhance recombination rates on ultrafast time scales, indicating that surface state mediated recombination is not a key loss pathway for either TiO2 polymorph. Rutile shows faster, and less intensity-dependent recombination than anatase, which we assign to its higher doping density. For both polymorphs, we conclude that bulk rather than surface recombination is the primary determinant of charge carrier lifetime.
C1 [Sachs, Michael; Pastor, Ernest; Durrant, James R.] Imperial Coll London, Dept Chem, South Kensington Campus, London SW7 2AZ, England.
[Kafizas, Andreas] UCL, Dept Chem, 20 Gordon St, London WC1H 0AJ, England.
[Pastor, Ernest] Lawrence Berkeley Natl Lab, Phys Biosci Div, Berkeley, CA 94720 USA.
RP Durrant, JR (reprint author), Imperial Coll London, Dept Chem, South Kensington Campus, London SW7 2AZ, England.
EM j.durrant@imperial.ac.uk
RI Kafizas, Andreas /B-2533-2010
OI Kafizas, Andreas /0000-0002-2282-4639
FU ERC AdG Intersolar [291482]; Imperial College; Engineering and Physical
Sciences Research Council (EPSRC); Ramsay Memorial Fellowships Trust
FX J.R.D. and M.S. acknowledge support from ERC AdG Intersolar (291482) and
the Imperial College Ph.D. Scholarship scheme. E.P. acknowledges the
Engineering and Physical Sciences Research Council (EPSRC) for funding.
A.K. thanks the Ramsay Memorial Fellowships Trust for funding.
NR 31
TC 0
Z9 0
U1 21
U2 21
PU AMER CHEMICAL SOC
PI WASHINGTON
PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA
SN 1948-7185
J9 J PHYS CHEM LETT
JI J. Phys. Chem. Lett.
PD OCT 6
PY 2016
VL 7
IS 19
BP 3742
EP 3746
DI 10.1021/acs.jpclett.6b01501
PG 5
WC Chemistry, Physical; Nanoscience & Nanotechnology; Materials Science,
Multidisciplinary; Physics, Atomic, Molecular & Chemical
SC Chemistry; Science & Technology - Other Topics; Materials Science;
Physics
GA DY3BT
UT WOS:000384966500006
PM 27564137
ER
PT J
AU Cherukara, MJ
Narayanan, B
Kinaci, A
Sasikumar, K
Gray, SK
Chan, MKY
Sankaranarayanan, SKRS
AF Cherukara, Mathew J.
Narayanan, Badri
Kinaci, Alper
Sasikumar, Kiran
Gray, Stephen K.
Chan, Maria K. Y.
Sankaranarayanan, Subramanian K. R. S.
TI Ab Initio-Based Bond Order Potential to Investigate Low Thermal
Conductivity of Stanene Nanostructures
SO JOURNAL OF PHYSICAL CHEMISTRY LETTERS
LA English
DT Article
ID TEMPERATURE-DEPENDENCE; ELECTRONIC-STRUCTURES; MOLECULAR-DYNAMICS;
CARBON NANOTUBES; FORCE-FIELD; GRAPHENE; GERMANENE; SILICENE;
NANOCLUSTERS; PHOSPHORENE
AB We introduce a bond order potential (BOP) for stanene based on an ab initio derived training data set. The potential is optimized to accurately describe the energetics, as well as thermal and mechanical properties of a free-standing sheet, and used to study diverse nanostructures of stanene, including tubes and ribbons. As a representative case study, using the potential, we perform molecular dynamics simulations to study stanene's structure and temperature-dependent thermal conductivity. We find that the structure of stanene is highly rippled, far in excess of other 2-D materials (e.g., graphene), owing to its low in-plane stiffness (stanene: similar to 25 N/m; graphene: similar to 480 N/m). The extent of stanene's rippling also shows stronger temperature dependence compared to that in graphene. Furthermore, we find that stanene based nanostructures have significantly lower thermal conductivity compared to graphene based structures owing to their softness (i.e., low phonon group velocities) and high anharmonic response. Our newly developed BOP will facilitate dimensional heterostructures for thermoelectric and thermal management applications. the exploration of stanene based low
C1 [Cherukara, Mathew J.] Argonne Natl Lab, Xray Sci Div, 9700 S Cass Ave, Argonne, IL 60439 USA.
[Narayanan, Badri; Kinaci, Alper; Sasikumar, Kiran; Gray, Stephen K.; Chan, Maria K. Y.; Sankaranarayanan, Subramanian K. R. S.] Argonne Natl Lab, Ctr Nanoscale Mat, 9700 S Cass Ave, Argonne, IL 60439 USA.
[Gray, Stephen K.; Chan, Maria K. Y.; Sankaranarayanan, Subramanian K. R. S.] Univ Chicago, Computat Inst, Chicago, IL 60637 USA.
RP Cherukara, MJ (reprint author), Argonne Natl Lab, Xray Sci Div, 9700 S Cass Ave, Argonne, IL 60439 USA.; Sankaranarayanan, SKRS (reprint author), Argonne Natl Lab, Ctr Nanoscale Mat, 9700 S Cass Ave, Argonne, IL 60439 USA.; Sankaranarayanan, SKRS (reprint author), Univ Chicago, Computat Inst, Chicago, IL 60637 USA.
EM mcherukara@aps.anl.gov; ssankaranarayanan@anl.gov
FU Argonne LDRD [2015-149-R1]; U.S. Department of Energy, Office of
Science, Office of Basic Energy Sciences [DE-AC02-06CH11357]; National
Science Foundation [ACI-1053575]; Office of Science of the U.S.
Department of Energy [DE-AC02-05CH11231]
FX This work was supported by Argonne LDRD 2015-149-R1 (Integrated Imaging,
Modeling, and Analysis of Ultrafast Energy Transport in Nanomaterials).
Use of the Center for Nanoscale Materials, an Office of Science user
facility, was supported by the U.S. Department of Energy, Office of
Science, Office of Basic Energy Sciences, under Contract No.
DE-AC02-06CH11357. This work used the Extreme Science and Engineering
Discovery Environment (XSEDE),60 which is supported by
National Science Foundation grant number ACI-1053575. This research used
resources of the National Energy Research Scientific computing Center, a
DOE Office of Science User Facility supported by the Office of Science
of the U.S. Department of Energy under Contract No. DE-AC02-05CH11231.
We gratefully acknowledge the computing resources provided on Blues, a
high-performance computing cluster operated by the Laboratory Computing
Resource Center at Argonne National Laboratory. We thank Ross J. Harder
at the Advanced Photon Source for many stimulating and motivating
discussions.
NR 58
TC 4
Z9 4
U1 22
U2 22
PU AMER CHEMICAL SOC
PI WASHINGTON
PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA
SN 1948-7185
J9 J PHYS CHEM LETT
JI J. Phys. Chem. Lett.
PD OCT 6
PY 2016
VL 7
IS 19
BP 3752
EP 3759
DI 10.1021/acs.jpclett.6b01562
PG 8
WC Chemistry, Physical; Nanoscience & Nanotechnology; Materials Science,
Multidisciplinary; Physics, Atomic, Molecular & Chemical
SC Chemistry; Science & Technology - Other Topics; Materials Science;
Physics
GA DY3BT
UT WOS:000384966500008
PM 27569053
ER
PT J
AU Grinter, DC
Remesal, ER
Luo, S
Evans, J
Senanayake, SD
Stacchiola, DJ
Graciani, J
Sanz, JF
Rodriguez, JA
AF Grinter, David C.
Remesal, Elena R.
Luo, Si
Evans, Jaime
Senanayake, Sanjaya D.
Stacchiola, Dario J.
Graciani, Jesus
Fernandez Sanz, Javier
Rodriguez, Jose A.
TI Potassium and Water Coadsorption on TiO2(110): OH-Induced Anchoring of
Potassium and the Generation of Single-Site Catalysts
SO JOURNAL OF PHYSICAL CHEMISTRY LETTERS
LA English
DT Article
ID AUGMENTED-WAVE METHOD; THEORETICAL-ANALYSIS; TIO2 SURFACES; ADSORPTION;
MECHANISM; METALS; SHIFT; GOLD; NANOPARTICLES; DISSOCIATION
AB Potassium deposition on TiO2(110) results in reduction of the substrate and formation of loosely bound potassium species that can move easily on the oxide surface to promote catalytic activity. The results of density functional calculations predict a large adsorption energy (similar to 3.2 eV) with a small barrier (similar to 0.25 eV) for diffusion on the oxide surface. In scanning tunneling microscopy images, the adsorbed alkali atoms lose their mobility when in contact with surface OH groups. Furthermore, K adatoms facilitate the dissociation of water on the titania surface. The K-(OH) species generated are good sites for the binding of gold clusters on the TiO2(110) surface, producing Au/K/TiO2(110) systems with high activity for the water-gas shift.
C1 [Grinter, David C.; Luo, Si; Senanayake, Sanjaya D.; Stacchiola, Dario J.; Rodriguez, Jose A.] Brookhaven Natl Lab, Dept Chem, Upton, NY 11973 USA.
[Remesal, Elena R.; Graciani, Jesus; Fernandez Sanz, Javier] Univ Seville, Dept Quim Fis, E-41012 Seville, Spain.
[Luo, Si; Rodriguez, Jose A.] SUNY Stony Brook, Dept Chem, Stony Brook, NY 11794 USA.
[Evans, Jaime] Cent Univ Venezuela, Fac Ciencias, Caracas 1020A, Venezuela.
RP Rodriguez, JA (reprint author), Brookhaven Natl Lab, Dept Chem, Upton, NY 11973 USA.; Sanz, JF (reprint author), Univ Seville, Dept Quim Fis, E-41012 Seville, Spain.; Rodriguez, JA (reprint author), SUNY Stony Brook, Dept Chem, Stony Brook, NY 11794 USA.
RI Senanayake, Sanjaya/D-4769-2009;
OI Senanayake, Sanjaya/0000-0003-3991-4232; Grinter,
David/0000-0001-6089-119X
FU U.S. Department of Energy, Chemical Sciences Division [DE-SC0012704];
Spanish Ministerio de Economia y Competitividad [CTQ2015-64669-P]; Junta
de Andalucia [P12-FQM-1595]
FX The experimental studies at Brookhaven National Laboratory were
supported by the U.S. Department of Energy, Chemical Sciences Division
(DE-SC0012704). The work performed at the University of Seville was
funded by the Spanish Ministerio de Economia y Competitividad, Grant
CTQ2015-64669-P, Junta de Andalucia, Grant P12-FQM-1595, and European
FEDER Computational resources were provided by the Barcelona
Supercomputing Center/Centro Nacional de Supercomputacion (Spain).
NR 40
TC 1
Z9 1
U1 19
U2 19
PU AMER CHEMICAL SOC
PI WASHINGTON
PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA
SN 1948-7185
J9 J PHYS CHEM LETT
JI J. Phys. Chem. Lett.
PD OCT 6
PY 2016
VL 7
IS 19
BP 3866
EP 3872
DI 10.1021/acs.jpclett.6b01623
PG 7
WC Chemistry, Physical; Nanoscience & Nanotechnology; Materials Science,
Multidisciplinary; Physics, Atomic, Molecular & Chemical
SC Chemistry; Science & Technology - Other Topics; Materials Science;
Physics
GA DY3BT
UT WOS:000384966500025
PM 27631665
ER
PT J
AU Rizzuto, AM
Irgen-Gioro, S
Eftekhari-Bafrooei, A
Saykally, RJ
AF Rizzuto, Anthony M.
Irgen-Gioro, Shawn
Eftekhari-Bafrooei, Ali
Saykally, Richard J.
TI Broadband Deep UV Spectra of Interfacial Aqueous Iodide
SO JOURNAL OF PHYSICAL CHEMISTRY LETTERS
LA English
DT Article
ID LIQUID WATER-SURFACE; REPULSIVE FORCES; GENERATION; SPECTROSCOPY;
ELECTROLYTES; ADSORPTION; DYNAMICS; CLUSTERS; ANIONS; HALIDE
AB The behavior of ions at aqueous interfaces influences vital processes in many fields but has long remained a subject of controversy. Over the past decade, counterintuitive surface concentration enhancement of several ions in aqueous solution has been demonstrated via nonlinear laser spectroscopy and mass spectrometry. While the evidence for significant ion enhancement at the air water interface is convincing, the mechanism remains incompletely understood. Toward this end, we present the full broadband DUV-SFG spectrum of the charge-transfer-to-solvent (CTTS) band of interfacial aqueous iodide measured in a single laser shot with a newly developed broadband deep UV-SFG technique, clearly revealing a similar to 8 nm redshift and a significant linewidthr narrowing relative to bulk solution spectra. KI and NaI solutions yield indistinguishable results. Additionally, we observe a dramatic change in the relative intensities of the J = 3/2 and 1/2 CTTS transitions.
C1 [Rizzuto, Anthony M.; Irgen-Gioro, Shawn; Eftekhari-Bafrooei, Ali; Saykally, Richard J.] Univ Calif Berkeley, Dept Chem, D31 Hildebrand Hall, Berkeley, CA 94720 USA.
[Rizzuto, Anthony M.; Eftekhari-Bafrooei, Ali; Saykally, Richard J.] Lawrence Berkeley Natl Lab, Div Chem Sci, Berkeley, CA 94720 USA.
[Irgen-Gioro, Shawn] Northwestern Univ, Dept Chem, 2145 Sheridan Rd, Evanston, IL 60208 USA.
[Eftekhari-Bafrooei, Ali] IMRA Amer, Applicat Dev Ctr, Fremont, CA 94582 USA.
RP Saykally, RJ (reprint author), Univ Calif Berkeley, Dept Chem, D31 Hildebrand Hall, Berkeley, CA 94720 USA.
EM saykally@berkeley.edu
FU Office of Basic Energy Sciences, Office of Science, U.S. Department of
Energy (DOE) through the Chemical Sciences Division of the Lawrence
Berkeley National Laboratory (LBNL) [DE-AC02-05CH11231]
FX This work was supported by the Director, Office of Basic Energy
Sciences, Office of Science, U.S. Department of Energy (DOE) under
Contract No. DE-AC02-05CH11231 through the Chemical Sciences Division of
the Lawrence Berkeley National Laboratory (LBNL).
NR 28
TC 1
Z9 1
U1 9
U2 9
PU AMER CHEMICAL SOC
PI WASHINGTON
PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA
SN 1948-7185
J9 J PHYS CHEM LETT
JI J. Phys. Chem. Lett.
PD OCT 6
PY 2016
VL 7
IS 19
BP 3882
EP 3885
DI 10.1021/acs.jpclett.6b01931
PG 4
WC Chemistry, Physical; Nanoscience & Nanotechnology; Materials Science,
Multidisciplinary; Physics, Atomic, Molecular & Chemical
SC Chemistry; Science & Technology - Other Topics; Materials Science;
Physics
GA DY3BT
UT WOS:000384966500027
PM 27635463
ER
PT J
AU Makinaga, A
Massarczyk, R
Beard, M
Schwengner, R
Otsu, H
Al-Abdullah, T
Anders, M
Bemmerer, D
Hannaske, R
John, R
Junghans, AR
Muller, SE
Roder, M
Schmidt, K
Wagner, A
AF Makinaga, A.
Massarczyk, R.
Beard, M.
Schwengner, R.
Otsu, H.
Al-Abdullah, T.
Anders, M.
Bemmerer, D.
Hannaske, R.
John, R.
Junghans, A. R.
Mueller, S. E.
Roeder, M.
Schmidt, K.
Wagner, A.
TI Dipole strength in Se-80 for s process and nuclear transmutation of
Se-79
SO PHYSICAL REVIEW C
LA English
DT Article
ID CAPTURE CROSS-SECTIONS; PROCESS NUCLEOSYNTHESIS; PHOTON-SCATTERING;
ISOTOPES; DENSITY; WIDTHS; MODEL; SIMULATION; RESONANCE; FORMULA
AB The dipole strength distribution of Se-80 was studied in a photon-scattering experiment by using bremsstrahlung produced with an electron beam of energy 11.5 MeV at the linear accelerator ELBE. We identified 180 gamma transitions up to an energy of 9.6 MeV, and analyzed the strength in the quasicontinuum of the spectrum. Simulations of statistical gamma-ray cascades were performed to estimate intensities of inelastic transitions and to correct the intensities of the ground-state transitions for their branching ratios. The photoabsorption cross section below the neutron-separation energy derived in this way was combined with the photoabsorption cross section obtained from an earlier (gamma,n) experiment and used as an input for the calculation of Se-79(n,gamma) reaction rates on the basis of the statistical reaction model.
C1 [Makinaga, A.] Hokkaido Univ, Fac Sci, Kita Ku, Kita 15,Nishi 7, Sapporo, Hokkaido 0608638, Japan.
[Makinaga, A.] JEIN Inst Fundamental Sci, Sakyo Ku, 5-14 Yoshida Honmachiu, Kyoto 6068317, Japan.
[Massarczyk, R.; Schwengner, R.; Anders, M.; Bemmerer, D.; Hannaske, R.; John, R.; Junghans, A. R.; Mueller, S. E.; Roeder, M.; Schmidt, K.; Wagner, A.] Helmholtz Zentrum Dresden Rossendorf, D-01328 Dresden, Germany.
[Beard, M.] Univ Notre Dame, Dept Phys, Notre Dame, IN 46556 USA.
[Otsu, H.] RIKEN Nishina Ctr, 2-1 Hirosawa, Wako, Saitama 3510198, Japan.
[Al-Abdullah, T.] Hashemite Univ, Zarqa, Jordan.
[Schmidt, K.] Tech Univ Dresden, D-01062 Dresden, Germany.
[Makinaga, A.] Hokkaido Univ, Grad Sch Med, Kita Ku, Kita 15,Nishi 7, Sapporo, Hokkaido 0608638, Japan.
[Massarczyk, R.] Los Alamos Natl Lab, Los Alamos, NM 87545 USA.
[Schmidt, K.] Michigan State Univ, Natl Superconducting Cyclotron Lab, E Lansing, MI 48824 USA.
RP Makinaga, A (reprint author), Hokkaido Univ, Fac Sci, Kita Ku, Kita 15,Nishi 7, Sapporo, Hokkaido 0608638, Japan.; Makinaga, A (reprint author), JEIN Inst Fundamental Sci, Sakyo Ku, 5-14 Yoshida Honmachiu, Kyoto 6068317, Japan.; Makinaga, A (reprint author), Hokkaido Univ, Grad Sch Med, Kita Ku, Kita 15,Nishi 7, Sapporo, Hokkaido 0608638, Japan.
RI Wagner, Andreas/G-3127-2013; Muller, Stefan/D-5431-2015; Junghans,
Arnd/D-4596-2012; Bemmerer, Daniel/C-9092-2013
OI Wagner, Andreas/0000-0001-7575-3961; Muller, Stefan/0000-0001-6273-7102;
Bemmerer, Daniel/0000-0003-0470-8367
FU Nuclear Astrophysics Virtual Institute (NAVI) [HGF VH-VI-417]
FX We thank the staff of the ELBE accelerator for the cooperation during
the experiment and A. Hartmann for technical assistance. Special thanks
are due to H. Utsunomiya for lending part of the 80Se
material. T.A.-A. was supported by the Nuclear Astrophysics Virtual
Institute (NAVI, HGF VH-VI-417).
NR 71
TC 0
Z9 0
U1 4
U2 4
PU AMER PHYSICAL SOC
PI COLLEGE PK
PA ONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA
SN 2469-9985
EI 2469-9993
J9 PHYS REV C
JI Phys. Rev. C
PD OCT 6
PY 2016
VL 94
IS 4
AR 044304
DI 10.1103/PhysRevC.94.044304
PG 10
WC Physics, Nuclear
SC Physics
GA DY6NS
UT WOS:000385244600003
ER
PT J
AU Zhao, PW
Ring, P
Meng, J
AF Zhao, P. W.
Ring, P.
Meng, J.
TI Configuration interaction in symmetry-conserving covariant density
functional theory
SO PHYSICAL REVIEW C
LA English
DT Article
ID ANGULAR-MOMENTUM PROJECTION; HARTREE-BOGOLIUBOV THEORY;
MEAN-FIELD-THEORY; HIGH-SPIN STATES; NUCLEAR-STRUCTURE; ANTIMAGNETIC
ROTATION; WAVE-FUNCTIONS; FINITE NUCLEI; SHELL-MODEL; MOTION
AB A new method to calculate spectroscopic properties of deformed nuclei is proposed: configuration interaction on top of projected density functional theory (CI-PDFT). The general concept of this approach is discussed in the framework of covariant density functional theory and its validity is illustrated in an application to the yrast band of the nucleus Cr-54. It is found that the experimentally observed excitation energies for the yrast band in Cr-54 can be well reproduced. In contrast to conventional shell-model calculations, there is no core and only a relatively small number of configurations is sufficient for a satisfying description. No new parameters are necessary, because the effective interaction is derived from an universal density functional given in the literature.
C1 [Zhao, P. W.] Argonne Natl Lab, Div Phys, Argonne, IL 60439 USA.
[Zhao, P. W.; Ring, P.; Meng, J.] Peking Univ, Sch Phys, State Key Lab Nucl Phys & Technol, Beijing 100871, Peoples R China.
[Ring, P.] Tech Univ Munich, Dept Phys, D-85747 Garching, Germany.
[Meng, J.] Beihang Univ, Sch Phys & Nucl Energy Engn, Beijing 100191, Peoples R China.
RP Zhao, PW (reprint author), Argonne Natl Lab, Div Phys, Argonne, IL 60439 USA.; Zhao, PW (reprint author), Peking Univ, Sch Phys, State Key Lab Nucl Phys & Technol, Beijing 100871, Peoples R China.
RI Zhao, Pengwei/F-9107-2010; Meng, Jie/B-8548-2009
OI Zhao, Pengwei/0000-0001-8243-2381; Meng, Jie/0000-0002-0977-5318
FU U.S. Department of Energy (DOE), Office of Science, Office of Nuclear
Physics [DE-AC02-06CH11357]; Chinese Major State 973 Program
[2013CB834400]; NSFC [11335002, 11621131001]; Laboratory Computing
Resource Center at Argonne National Laboratory; DFG Cluster of
Excellence "Origin and Structure of the Universe"
FX We thank R. V. F. Janssens and Robert B. Wiringa for careful reading of
the manuscript. This work is supported by U.S. Department of Energy
(DOE), Office of Science, Office of Nuclear Physics, under Contract No.
DE-AC02-06CH11357, by the Chinese Major State 973 Program 2013CB834400,
and by the NSFC Grants No. 11335002 and No. 11621131001. We also
acknowledge support from the Laboratory Computing Resource Center at
Argonne National Laboratory, and the DFG Cluster of Excellence "Origin
and Structure of the Universe" (www.universe-cluster.de).
NR 62
TC 0
Z9 0
U1 3
U2 3
PU AMER PHYSICAL SOC
PI COLLEGE PK
PA ONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA
SN 2469-9985
EI 2469-9993
J9 PHYS REV C
JI Phys. Rev. C
PD OCT 6
PY 2016
VL 94
IS 4
AR 041301
DI 10.1103/PhysRevC.94.041301
PG 6
WC Physics, Nuclear
SC Physics
GA DY6NS
UT WOS:000385244600001
ER
PT J
AU Liu, Y
Chen, LL
Hilliard, D
Huang, QS
Liu, F
Wang, M
Bottger, R
Hubner, R
N'Diaye, AT
Arenholz, E
Heera, V
Skorupa, W
Zhou, SQ
AF Liu, Yu
Chen, Lianlian
Hilliard, Donovan
Huang, Qing-song
Liu, Fang
Wang, Mao
Boettger, Roman
Huebner, Rene
N'Diaye, Alpha T.
Arenholz, Elke
Heera, Viton
Skorupa, Wolfgang
Zhou, Shengqiang
TI Controllable growth of vertically aligned graphene on C-face SiC
SO SCIENTIFIC REPORTS
LA English
DT Article
ID LITHIUM-ION BATTERIES; HIGH-PERFORMANCE; SILICON-CARBIDE; ELECTRODES;
SHEETS; RECRYSTALLIZATION; IMPLANTATION; FABRICATION; BEHAVIOR
AB We investigated how to control the growth of vertically aligned graphene on C-face SiC by varying the processing conditions. It is found that, the growth rate scales with the annealing temperature and the graphene height is proportional to the annealing time. Temperature gradient and crystalline quality of the SiC substrates influence their vaporization. The partial vapor pressure is crucial as it can interfere with further vaporization. A growth mechanism is proposed in terms of physical vapor transport. The monolayer character of vertically aligned graphene is verified by Raman and X-ray absorption spectroscopy. With the processed samples, d(0) magnetism is realized and negative magnetoresistance is observed after Cu implantation. We also prove that multiple carriers exist in vertically aligned graphene.
C1 [Liu, Yu; Hilliard, Donovan; Liu, Fang; Wang, Mao; Boettger, Roman; Huebner, Rene; Heera, Viton; Skorupa, Wolfgang; Zhou, Shengqiang] Helmholtz Zentrum Dresden Rossendorf, Inst Ion Beam Phys & Mat Res, D-01328 Dresden, Germany.
[Chen, Lianlian] Beijing Informat Sci & Technol Univ, Dept Basic Sci, Beijing 100192, Peoples R China.
[Hilliard, Donovan] Dublin Inst Technol, Sch Phys, Dublin, Ireland.
[Huang, Qing-song] Sichuan Univ, Sch Chem Engn, Chengdu 610065, Peoples R China.
[Liu, Fang; Wang, Mao] Tech Univ Dresden, D-01062 Dresden, Germany.
[N'Diaye, Alpha T.; Arenholz, Elke] Lawrence Berkeley Natl Lab, Adv Light Source, Berkeley, CA 94720 USA.
RP Liu, Y (reprint author), Helmholtz Zentrum Dresden Rossendorf, Inst Ion Beam Phys & Mat Res, D-01328 Dresden, Germany.
EM y.liu@hzdr.de
RI Zhou, Shengqiang/C-1497-2009; Liu, Yu/A-1018-2012
OI Zhou, Shengqiang/0000-0002-4885-799X;
FU Ion Beam Center (IBC) at HZDR; Office of Science, Office of Basic Energy
Sciences, of the US Department of Energy [DE-AC02-05CH11231]; Helmholtz
Postdoc Programme (Initiative and Networking Fund) [PD-146]
FX Yu Liu would like to thank Christian Frenzel and Ilona Skorupa from HZDR
for equipment maintenance, Elfi Christalle from HZDR for SEM imaging,
Zhilin Li, Dr. Jiao Huang, Prof. Liwei Guo from Institute of Physics,
CAS for the fruitful discussion about vertical graphene, Dr. Jie Shen
from TU Delft for the assistance in transport measurements and Dr.
Chunjun Liu from TankeBlue Semiconductor Co. Ltd. for designing the
graphite susceptors and mounts. Support by the Ion Beam Center (IBC) at
HZDR is gratefully acknowledged. The Advanced Light Source is supported
by the Director, Office of Science, Office of Basic Energy Sciences, of
the US Department of Energy under Contract No. DE-AC02-05CH11231. The
work is financially supported by the Helmholtz Postdoc Programme
(Initiative and Networking Fund, PD-146).
NR 46
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Z9 0
U1 49
U2 49
PU NATURE PUBLISHING GROUP
PI LONDON
PA MACMILLAN BUILDING, 4 CRINAN ST, LONDON N1 9XW, ENGLAND
SN 2045-2322
J9 SCI REP-UK
JI Sci Rep
PD OCT 6
PY 2016
VL 6
AR 34814
DI 10.1038/srep34814
PG 10
WC Multidisciplinary Sciences
SC Science & Technology - Other Topics
GA DY0DJ
UT WOS:000384766800001
PM 27708399
ER
PT J
AU Bernstein, A
Sargent, EH
Aspuru-Guzik, A
Cogdell, R
Fleming, GR
Van Grondelle, R
Molina, M
AF Bernstein, Alan
Sargent, Edward H.
Aspuru-Guzik, Alan
Cogdell, Richard
Fleming, Graham R.
Van Grondelle, Rienk
Molina, Mario
TI Renewables need a grand-challenge strategy
SO NATURE
LA English
DT Editorial Material
C1 [Bernstein, Alan] Canadian Inst Adv Res CIFAR, Toronto, ON, Canada.
[Sargent, Edward H.] Univ Toronto, Toronto, ON M5S 1A1, Canada.
[Sargent, Edward H.] Univ Toronto, Edward S Rogers Sr Dept Elect & Comp Engn, CIFARs Bioinspired Solar Energy Program, Toronto, ON M5S 1A1, Canada.
[Aspuru-Guzik, Alan] Harvard Univ, Cambridge, MA 02138 USA.
[Aspuru-Guzik, Alan] Harvard Univ, Chem & Chem Biol, Cambridge, MA 02138 USA.
[Cogdell, Richard] Univ Glasgow, Glasgow, Lanark, Scotland.
[Cogdell, Richard] Univ Glasgow, Bot, Glasgow, Lanark, Scotland.
[Fleming, Graham R.] Univ Calif Berkeley, Kavli Energy NanoSci Inst, Chem, Berkeley, CA 94720 USA.
[Fleming, Graham R.] Lawrence Berkeley Natl Lab, Berkeley, CA USA.
[Van Grondelle, Rienk] Vrije Univ Amsterdam, Amsterdam, Netherlands.
[Van Grondelle, Rienk] Vrije Univ Amsterdam, Biophys, Amsterdam, Netherlands.
[Molina, Mario] Univ Calif San Diego, Dept Chem & Biochem, San Diego, CA 92103 USA.
[Molina, Mario] Mario Molina Ctr Strateg Studies Energy & Environ, Mexico City, DF, Mexico.
RP Aspuru-Guzik, A (reprint author), Harvard Univ, Cambridge, MA 02138 USA.; Aspuru-Guzik, A (reprint author), Harvard Univ, Chem & Chem Biol, Cambridge, MA 02138 USA.
EM alan.bernstein@cifar.ca
NR 2
TC 0
Z9 0
U1 26
U2 26
PU NATURE PUBLISHING GROUP
PI LONDON
PA MACMILLAN BUILDING, 4 CRINAN ST, LONDON N1 9XW, ENGLAND
SN 0028-0836
EI 1476-4687
J9 NATURE
JI Nature
PD OCT 6
PY 2016
VL 538
IS 7623
BP 30
EP 30
PG 1
WC Multidisciplinary Sciences
SC Science & Technology - Other Topics
GA DX8LD
UT WOS:000384638900014
ER
PT J
AU Choueiri, RM
Galati, E
Therien-Aubin, H
Klinkova, A
Larin, EM
Querejeta-Fernandez, A
Han, LL
Xin, HL
Gang, O
Zhulina, EB
Rubinstein, M
Kumacheva, E
AF Choueiri, Rachelle M.
Galati, Elizabeth
Therien-Aubin, Heloise
Klinkova, Anna
Larin, Egor M.
Querejeta-Fernandez, Ana
Han, Lili
Xin, Huolin L.
Gang, Oleg
Zhulina, Ekaterina B.
Rubinstein, Michael
Kumacheva, Eugenia
TI Surface patterning of nanoparticles with polymer patches
SO NATURE
LA English
DT Article
ID INORGANIC NANOPARTICLES; JANUS NANOPARTICLES; LIGAND SHELL; PARTICLES;
INTERFACE; SOLVENTS; COLLOIDS; BRUSHES; CHAINS
AB Patterning of colloidal particles with chemically or topographically distinct surface domains (patches) has attracted intense research interest(1-3). Surface-patterned particles act as colloidal analogues of atoms and molecules(4,5), serve as model systems in studies of phase transitions in liquid systems(6), behave as 'colloidal surfactants'(7) and function as templates for the synthesis of hybrid particles(8). The generation of micrometre- and submicrometre-sized patchy colloids is now efficient(9-11), but surface patterning of inorganic colloidal nanoparticles with dimensions of the order of tens of nanometres is uncommon. Such nanoparticles exhibit size-and shape-dependent optical, electronic and magnetic properties, and their assemblies show new collective properties(12). At present, nanoparticle patterning is limited to the generation of two-patch nanoparticles(13-15), and nanoparticles with surface ripples(16) or a 'raspberry' surface morphology(17). Here we demonstrate nanoparticle surface patterning, which utilizes thermodynamically driven segregation of polymer ligands from a uniform polymer brush into surface-pinned micelles following a change in solvent quality. Patch formation is reversible but can be permanently preserved using a photocrosslinking step. The methodology offers the ability to control the dimensions of patches, their spatial distribution and the number of patches per nanoparticle, in agreement with a theoretical model. The versatility of the strategy is demonstrated by patterning nanoparticles with different dimensions, shapes and compositions, tethered with various types of polymers and subjected to different external stimuli. These patchy nanocolloids have potential applications in fundamental research, the self-assembly of nanomaterials, diagnostics, sensing and colloidal stabilization.
C1 [Choueiri, Rachelle M.; Galati, Elizabeth; Therien-Aubin, Heloise; Klinkova, Anna; Larin, Egor M.; Querejeta-Fernandez, Ana; Kumacheva, Eugenia] Univ Toronto, Dept Chem, 80 St George St, Toronto, ON M5S 3H6, Canada.
[Han, Lili; Xin, Huolin L.; Gang, Oleg] Brookhaven Natl Lab, Ctr Funct Nanomat, Upton, NY 11973 USA.
[Han, Lili] Tianjin Univ, Inst New Energy Mat, Sch Mat Sci & Engn, Tianjin 300072, Peoples R China.
[Zhulina, Ekaterina B.] Russian Acad Sci, Inst Macromol Cpds, St Petersburg 199004, Russia.
[Zhulina, Ekaterina B.] St Petersburg Natl Univ Informat Technol Mech & O, St Petersburg 197101, Russia.
[Rubinstein, Michael] Univ N Carolina, Dept Chem, Chapel Hill, NC 27599 USA.
[Kumacheva, Eugenia] Univ Toronto, Inst Biomat & Biomed Engn, 4 Taddle Creek Rd, Toronto, ON M5S 3G9, Canada.
[Kumacheva, Eugenia] Univ Toronto, Dept Chem Engn & Appl Chem, 200 Coll St, Toronto, ON M5S 3E5, Canada.
[Gang, Oleg] Columbia Univ, Dept Chem Engn, New York, NY 10027 USA.
[Gang, Oleg] Columbia Univ, Dept Appl Phys & Appl Math, New York, NY 10027 USA.
RP Kumacheva, E (reprint author), Univ Toronto, Dept Chem, 80 St George St, Toronto, ON M5S 3H6, Canada.; Kumacheva, E (reprint author), Univ Toronto, Inst Biomat & Biomed Engn, 4 Taddle Creek Rd, Toronto, ON M5S 3G9, Canada.; Kumacheva, E (reprint author), Univ Toronto, Dept Chem Engn & Appl Chem, 200 Coll St, Toronto, ON M5S 3E5, Canada.
EM ekumache@chem.utoronto.ca
RI Zhulina, Ekaterina/G-5177-2011;
OI Querejeta-Fernandez, Ana/0000-0002-9900-5367
FU Connaught Foundation; National Science and Engineering Research Council
of Canada; Russian Foundation for Basic Research [14-03-00372a];
Government of Russian Federation [074-U01]; National Science Foundation
[DMR-1309892, DMR-1436201, DMR-1121107]; National Institutes of Health
[P01-HL108808, 1UH2HL123645]; Cystic Fibrosis Foundation; US Department
of Energy, Office of Basic Energy Sciences [DE-SC0012704]; Natural
Sciences and Engineering Research Council of Canada
FX We thank the Connaught Foundation and the National Science and
Engineering Research Council of Canada (Discovery and Canada Research
Chair programmes) for financial support of this work. E.B.Z.
acknowledges partial support from the Russian Foundation for Basic
Research (grant 14-03-00372a) and from the Government of Russian
Federation (grant 074-U01). M.R. acknowledges financial support from the
National Science Foundation (grants DMR-1309892, DMR-1436201 and
DMR-1121107), the National Institutes of Health (grants P01-HL108808 and
1UH2HL123645), and the Cystic Fibrosis Foundation. Research was in part
carried out at the Center for Functional Nanomaterials, Brookhaven
National Laboratory supported by the US Department of Energy, Office of
Basic Energy Sciences (under contract number DE-SC0012704). R.M.C.
acknowledges the Natural Sciences and Engineering Research Council of
Canada for a PGS-D scholarship. A.K. acknowledges an Ontario Trillium
Scholarship. We thank M. Michaelis and S. Lin for initiating preliminary
experiments and I. Gourevich for help with imaging experiments.
NR 32
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PI LONDON
PA MACMILLAN BUILDING, 4 CRINAN ST, LONDON N1 9XW, ENGLAND
SN 0028-0836
EI 1476-4687
J9 NATURE
JI Nature
PD OCT 6
PY 2016
VL 538
IS 7623
BP 79
EP 83
DI 10.1038/nature19089
PG 5
WC Multidisciplinary Sciences
SC Science & Technology - Other Topics
GA DX8LD
UT WOS:000384638900037
PM 27556943
ER
PT J
AU Singappuli-Arachchige, D
Manzano, JS
Sherman, LM
Slowing, II
AF Singappuli-Arachchige, Dilini
Manzano, J. Sebastian
Sherman, Lindy M.
Slowing, Igor I.
TI Polarity Control at Interfaces: Quantifying Pseudo-solvent Effects in
Nano-confined Systems
SO CHEMPHYSCHEM
LA English
DT Article
DE confinement effects; mesoporous materials; molecular environments;
solvent effects; surface functionalization
ID AEROBIC ALCOHOL OXIDATION; SELF-ASSEMBLED MONOLAYERS; MESOPOROUS
SILICAS; HETEROGENEOUS CATALYSTS; CARBON MATERIALS; FUNCTIONALIZATION;
PYRENE; MODEL; NANOPARTICLES; FLUORESCENCE
AB Surface functionalization controls local environments and induces solvent-like effects at liquid-solid interfaces. We explored structure-property relationships between organic groups bound to pore surfaces of mesoporous silica nanoparticles and Stokes shifts of the adsorbed solvatochromic dye Prodan. Correlating shifts of the dye on the surfaces with its shifts in solvents resulted in a local polarity scale for functionalized pores. The scale was validated by studying the effects of pore polarity on quenching of Nile Red fluorescence and on the vibronic band structure of pyrene. Measurements were done in aqueous suspensions of porous particles, proving that the dielectric properties in the pores are different from the bulk solvent. The precise control of pore polarity was used to enhance the catalytic activity of TEMPO in the aerobic oxidation of furfuryl alcohol in water. An inverse relationship was found between pore polarity and activity of TEMPO in the pores, demonstrating that controlling the local polarity around an active site allows modulating the activity of nanoconfined catalysts.
C1 [Singappuli-Arachchige, Dilini; Manzano, J. Sebastian; Slowing, Igor I.] US DOE, Program Chem & Biol Sci, Ames Lab, 311 TASF, Ames, IA 50011 USA.
[Singappuli-Arachchige, Dilini; Manzano, J. Sebastian; Sherman, Lindy M.; Slowing, Igor I.] Iowa State Univ, Dept Chem, 1605 Gilman Hall, Ames, IA 50011 USA.
RP Slowing, II (reprint author), US DOE, Program Chem & Biol Sci, Ames Lab, 311 TASF, Ames, IA 50011 USA.; Slowing, II (reprint author), Iowa State Univ, Dept Chem, 1605 Gilman Hall, Ames, IA 50011 USA.
EM islowing@iastate.edu
OI Slowing, Igor/0000-0002-9319-8639
FU U.S. Department of Energy, Office of Basic Energy Sciences, Division of
Chemical Sciences, Geosciences, and Biosciences, through the Ames
Laboratory Catalysis Science program; U.S. Department of Energy
[DE-AC02-07CH11358]
FX This research is supported by the U.S. Department of Energy, Office of
Basic Energy Sciences, Division of Chemical Sciences, Geosciences, and
Biosciences, through the Ames Laboratory Catalysis Science program. The
Ames Laboratory is operated for the U.S. Department of Energy by Iowa
State University under Contract No. DE-AC02-07CH11358.
NR 47
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U1 12
U2 12
PU WILEY-V C H VERLAG GMBH
PI WEINHEIM
PA POSTFACH 101161, 69451 WEINHEIM, GERMANY
SN 1439-4235
EI 1439-7641
J9 CHEMPHYSCHEM
JI ChemPhysChem
PD OCT 5
PY 2016
VL 17
IS 19
BP 2982
EP 2986
DI 10.1002/cphc.201600740
PG 5
WC Chemistry, Physical; Physics, Atomic, Molecular & Chemical
SC Chemistry; Physics
GA EA7DW
UT WOS:000386790100006
PM 27429163
ER
PT J
AU Abbott, L
AF Abbott, Larry
TI Larry Abbott
SO NEURON
LA English
DT Editorial Material
AB Larry Abbott worked in theoretical physics before switching to theoretical neuroscience. In an interview with Neuron, he talks about his current interests, highlights recent developments in the acquisition of large amounts of neural activity data, and discusses the challenges associated with providing a cohesive understanding of the brain.
C1 [Abbott, Larry] Columbia Univ, Theoret Neurosci, New York, NY 10027 USA.
[Abbott, Larry] Stanford Linear Accelerator Ctr, Menlo Pk, CA USA.
[Abbott, Larry] CERN, Geneva, Switzerland.
[Abbott, Larry] Brandeis, Waltham, MA USA.
RP Abbott, L (reprint author), Columbia Univ, Theoret Neurosci, New York, NY 10027 USA.
NR 0
TC 0
Z9 0
U1 0
U2 0
PU CELL PRESS
PI CAMBRIDGE
PA 600 TECHNOLOGY SQUARE, 5TH FLOOR, CAMBRIDGE, MA 02139 USA
SN 0896-6273
EI 1097-4199
J9 NEURON
JI Neuron
PD OCT 5
PY 2016
VL 92
IS 1
BP 9
EP 10
DI 10.1016/j.neuron.2016.09.041
PG 2
WC Neurosciences
SC Neurosciences & Neurology
GA EA6TA
UT WOS:000386760700004
ER
PT J
AU Silberberg, SN
Taher, L
Lindtner, S
Sandberg, M
Nord, AS
Vogt, D
Mckinsey, GL
Hoch, R
Pattabiraman, K
Zhang, DJ
Ferran, JL
Rajkovic, A
Golonzhka, O
Kim, C
Zeng, HK
Puelles, L
Visel, A
Rubenstein, JLR
AF Silberberg, Shanni N.
Taher, Leila
Lindtner, Susan
Sandberg, Magnus
Nord, Alex S.
Vogt, Daniel
Mckinsey, Gabriel L.
Hoch, Renee
Pattabiraman, Kartik
Zhang, Dongji
Ferran, Jose L.
Rajkovic, Aleksandar
Golonzhka, Olga
Kim, Carol
Zeng, Hongkui
Puelles, Luis
Visel, Axel
Rubenstein, John L. R.
TI Subpallial Enhancer Transgenic Lines: a Data and Tool Resource to Study
Transcriptional Regulation of GABAergic Cell Fate
SO NEURON
LA English
DT Article
ID MEDIAL GANGLIONIC EMINENCE; CORTICAL INTERNEURONS; VENTRAL
TELENCEPHALON; MAMMALIAN BRAIN; CEREBRAL-CORTEX; EXPRESSION;
DIFFERENTIATION; MIGRATION; SUBTYPES; MASH1
AB Elucidating the transcriptional circuitry controlling forebrain development requires an understanding of enhancer activity and regulation. We generated stable transgenic mouse lines that express CreER(T2) and GFP from ten different enhancer elements with activity in distinct domains within the embryonic basal ganglia. We used these unique tools to generate a comprehensive regional fate map of the mouse subpallium, including sources for specific subtypes of amygdala neurons. We then focused on deciphering transcriptional mechanisms that control enhancer activity. Using machine-learning computations, in vivo chromosomal occupancy of 13 transcription factors that regulate subpallial patterning and differentiation and analysis of enhancer activity in Dlx1/2 and Lhx6 mutants, we elucidated novel molecular mechanisms that regulate region-specific enhancer activity in the developing brain. Thus, these subpallial enhancer transgenic lines are data and tool resources to study transcriptional regulation of GABAergic cell fate.
C1 [Silberberg, Shanni N.; Lindtner, Susan; Sandberg, Magnus; Vogt, Daniel; Mckinsey, Gabriel L.; Hoch, Renee; Pattabiraman, Kartik; Zhang, Dongji; Golonzhka, Olga; Kim, Carol; Rubenstein, John L. R.] Univ Calif San Francisco, Dept Psychiat, Program Neurosci, Rock Hall, San Francisco, CA 94158 USA.
[Taher, Leila] Univ Erlangen Nurnberg, Dept Biol, Div Bioinformat, D-91054 Erlangen, Germany.
[Nord, Alex S.; Visel, Axel] Lawrence Berkeley Natl Lab, Dept Funct Genom, MS 84-171, Berkeley, CA 94720 USA.
[Nord, Alex S.; Visel, Axel] US DOE, Joint Genome Inst, Walnut Creek, CA 94598 USA.
[Nord, Alex S.] Univ Calif Davis, Ctr Neurosci, Davis, CA 95618 USA.
[Hoch, Renee] PLOS, 1160 Battery St, San Francisco, CA 94111 USA.
[Ferran, Jose L.; Puelles, Luis] Univ Murcia, Fac Med, Dept Anat, E-30100 Murcia, Spain.
[Ferran, Jose L.; Puelles, Luis] IMIB, Murcia 30100, Spain.
[Rajkovic, Aleksandar] Magee Womens Res Inst, 204 Craft Ave, Pittsburgh, PA 15213 USA.
[Golonzhka, Olga] Acetylon Pharmaceut Inc, Boston, MA 02210 USA.
[Zeng, Hongkui] Allen Inst Brain Sci, Seattle, WA 98103 USA.
[Visel, Axel] Univ Calif Merced, Sch Nat Sci, Merced, CA 95343 USA.
RP Rubenstein, JLR (reprint author), Univ Calif San Francisco, Dept Psychiat, Program Neurosci, Rock Hall, San Francisco, CA 94158 USA.
EM john.rubenstein@ucsf.edu
RI Visel, Axel/A-9398-2009; Ferran, Jose/H-6288-2011
OI Visel, Axel/0000-0002-4130-7784; Ferran, Jose/0000-0002-3413-9452
FU Nina Ireland, Weston Havens Foundation; Allen Institute for Brain
Science; NIMH [R01 MH081880, R37 MH049428]; Spanish MICINN grant (EDR)
[BFU2014-57516P]; NIH [R01HG003988, U54HG006997]; Department of Energy,
University of California [DE-AC02-05CH11231]; [T32 GM007449]
FX This work was supported by the following research grants: to S.N.S., T32
GM007449; to J.L.R.R., Nina Ireland, Weston Havens Foundation, Allen
Institute for Brain Science, NIMH R01 MH081880, and NIMH R37 MH049428;
to L.P. and J.L.F., Spanish MICINN grant BFU2014-57516P (with EDR fund
support); and to A.V., NIH grants R01HG003988 and U54HG006997. Research
conducted at the E.O. Lawrence Berkeley National Laboratory was
performed under Department of Energy Contract DE-AC02-05CH11231,
University of California. J.L.R.R. is a Founder and Advisor for Neurona
Therapeutics.
NR 49
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Z9 0
U1 3
U2 3
PU CELL PRESS
PI CAMBRIDGE
PA 600 TECHNOLOGY SQUARE, 5TH FLOOR, CAMBRIDGE, MA 02139 USA
SN 0896-6273
EI 1097-4199
J9 NEURON
JI Neuron
PD OCT 5
PY 2016
VL 92
IS 1
BP 59
EP 74
DI 10.1016/j.neuron.2016.09.027
PG 16
WC Neurosciences
SC Neurosciences & Neurology
GA EA6TA
UT WOS:000386760700010
PM 27710791
ER
PT J
AU Levitz, J
Habrian, C
Bharill, S
Fu, Z
Vafabakhsh, R
Isacoff, EY
AF Levitz, Joshua
Habrian, Chris
Bharill, Shashank
Fu, Zhu
Vafabakhsh, Reza
Isacoff, Ehud Y.
TI Mechanism of Assembly and Cooperativity of Homomeric and Heteromeric
Metabotropic Glutamate Receptors
SO NEURON
LA English
DT Article
ID PROTEIN-COUPLED RECEPTOR; LIGAND-INDUCED REARRANGEMENT; CONFORMATIONAL
DYNAMICS; ACTIVATION MECHANISMS; STRUCTURAL BASIS; MESSENGER-RNA; GPCR
DIMERS; BINDING; DOMAIN; IDENTIFICATION
AB G protein-coupled receptors (GPCRs) mediate cellular responses to a wide variety of extracellular stimuli. GPCR dimerization may expand signaling diversity and tune functionality, but little is known about the mechanisms of subunit assembly and interaction or the signaling properties of heteromers. Using single-molecule subunit counting on class C metabotropic glutamate receptors (mGluRs), we map dimerization determinants and define a heterodimerization profile. Intersubunit fluorescence resonance energy transfer measurements reveal that interactions between ligand-binding domains control the conformational rearrangements underlying receptor activation. Selective liganding with photo-switchable tethered agonists conjugated to one or both subunits of covalently linked mGluR2 homodimers reveals that receptor activation is highly cooperative. Strikingly, this cooperativity is asymmetric in mGluR2/mGluR3 heterodimers. Our results lead to a model of cooperative activation of mGluRs that provides a framework for understanding how class C GPCRs couple extracellular binding to dimer reorganization and G protein activation.
C1 [Levitz, Joshua; Habrian, Chris; Bharill, Shashank; Fu, Zhu; Vafabakhsh, Reza; Isacoff, Ehud Y.] Univ Calif Berkeley, Dept Mol & Cell Biol, 229 Stanley Hall, Berkeley, CA 94720 USA.
[Levitz, Joshua; Habrian, Chris; Isacoff, Ehud Y.] Univ Calif Berkeley, Biophys Grad Grp, Berkeley, CA 94720 USA.
[Isacoff, Ehud Y.] Univ Calif Berkeley, Helen Wills Neurosci Inst, Berkeley, CA 94720 USA.
[Isacoff, Ehud Y.] Lawrence Berkeley Natl Lab, Biosci Div, Berkeley, CA 94720 USA.
[Levitz, Joshua] Weill Cornell Med Coll, Dept Biochem, 1300 York Ave, New York, NY 10065 USA.
RP Isacoff, EY (reprint author), Univ Calif Berkeley, Dept Mol & Cell Biol, 229 Stanley Hall, Berkeley, CA 94720 USA.; Isacoff, EY (reprint author), Univ Calif Berkeley, Biophys Grad Grp, Berkeley, CA 94720 USA.; Isacoff, EY (reprint author), Univ Calif Berkeley, Helen Wills Neurosci Inst, Berkeley, CA 94720 USA.; Isacoff, EY (reprint author), Lawrence Berkeley Natl Lab, Biosci Div, Berkeley, CA 94720 USA.
EM ehud@berkeley.edu
FU National Institutes of Health Nanomedicine Center for the Optical
Control of Biological Function [2PN2EY018241]; National Science
Foundation Major Research Instrumentation Award [1041078]; EAGER award
[IOS-1451027]; [S10 RR028971]
FX We thank A. Reiner for helpful discussion; M. Kienzler, J. Broichhagen,
A. Damijoinatas, and P. Leippe for chemical synthesis; and R. Arant, H.
Okada, and C. Stanley for technical assistance. The work was supported
by the National Institutes of Health Nanomedicine Center for the Optical
Control of Biological Function (2PN2EY018241) and instrumentation award
(S10 RR028971) and the National Science Foundation Major Research
Instrumentation Award (1041078) and EAGER award (IOS-1451027).
NR 63
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U1 8
U2 8
PU CELL PRESS
PI CAMBRIDGE
PA 600 TECHNOLOGY SQUARE, 5TH FLOOR, CAMBRIDGE, MA 02139 USA
SN 0896-6273
EI 1097-4199
J9 NEURON
JI Neuron
PD OCT 5
PY 2016
VL 92
IS 1
BP 143
EP 159
DI 10.1016/j.neuron.2016.08.036
PG 17
WC Neurosciences
SC Neurosciences & Neurology
GA EA6TA
UT WOS:000386760700017
PM 27641494
ER
PT J
AU Nian, L
Gao, K
Liu, F
Kan, YY
Jiang, XF
Liu, LL
Xie, ZQ
Peng, XB
Russell, TP
Ma, YG
AF Nian, Li
Gao, Ke
Liu, Feng
Kan, Yuanyuan
Jiang, Xiaofang
Liu, Linlin
Xie, Zengqi
Peng, Xiaobin
Russell, Thomas P.
Ma, Yuguang
TI 11% Efficient Ternary Organic Solar Cells with High Composition
Tolerance via Integrated Near-IR Sensitization and Interface Engineering
SO ADVANCED MATERIALS
LA English
DT Article
DE composition tolerance; high efficiency; near-IR sensitization;
photoconductive cathode interlayers; ternary organic solar cells
ID OPEN-CIRCUIT VOLTAGE; POWER CONVERSION EFFICIENCY; CONJUGATED POLYMER;
THERMAL-STABILITY; BANDGAP POLYMER; ENERGY-TRANSFER; SMALL MOLECULES;
FULLERENE; BISADDUCT; ACCEPTOR
AB Highly efficient electron extraction is achieved by using a photoconductive cathode interlayer in inverted ternary organic solar cells (OSCs) where a near-IR absorbing porphyrin molecule is used as the sensitizer. The OSCs show improved device performance when the ratio of the two donors varies in a large region and a maximum power conversion efficiency up to 11.03% is demonstrated.
C1 [Nian, Li; Gao, Ke; Kan, Yuanyuan; Jiang, Xiaofang; Liu, Linlin; Xie, Zengqi; Peng, Xiaobin; Ma, Yuguang] South China Univ Technol, Inst Polymer Optoelect Mat & Devices, State Key Lab Luminescent Mat & Devices, Guangzhou 510640, Guangdong, Peoples R China.
[Liu, Feng] Shanghai Jiao Tong Univ, Dept Phys & Astron, Shanghai 200240, Peoples R China.
[Liu, Feng; Russell, Thomas P.] Lawrence Berkeley Natl Lab, Div Mat Sci, Berkeley, CA 94720 USA.
[Russell, Thomas P.] Univ Massachusetts, Dept Polymer Sci & Engn, Amherst, MA 01003 USA.
RP Xie, ZQ; Peng, XB (reprint author), South China Univ Technol, Inst Polymer Optoelect Mat & Devices, State Key Lab Luminescent Mat & Devices, Guangzhou 510640, Guangdong, Peoples R China.; Russell, TP (reprint author), Lawrence Berkeley Natl Lab, Div Mat Sci, Berkeley, CA 94720 USA.; Russell, TP (reprint author), Univ Massachusetts, Dept Polymer Sci & Engn, Amherst, MA 01003 USA.
EM msxiez@scut.edu.cn; chxbpeng@scut.edu.cn; russell@mail.pse.umass.edu
RI Xie, Zengqi/H-5296-2013; Gao, Ke/B-3412-2017; Liu, Feng/J-4361-2014
OI Liu, Feng/0000-0002-5572-8512
FU National Basic Research Program of China (973 Program) [2014CB643504];
National Natural Science Foundation of China [51373054, 51573055,
51521002, 21334002]; Fundamental Research Funds for the Central
Universities; Introduced Innovative R&D Team of Guangdong
[201101C0105067115]; International Science & Technology Cooperation
Program of China [2013DFG52740, 2010DFA52150]; Natural Science
Foundation of China [51473053, 51073060]; U.S. Office of Naval Research
[N00014-15-1-2244]; DOE, Office of Science, and Office of Basic Energy
Sciences
FX L.N. and K.G. contributed equally to this work. Z. Xie and Y. Ma were
supported by the National Basic Research Program of China (973 Program)
(2014CB643504), the National Natural Science Foundation of China (Grant
Nos. 51373054, 51573055, 51521002, and 21334002), Fundamental Research
Funds for the Central Universities, and Introduced Innovative R&D Team
of Guangdong (Grant No. 201101C0105067115). X. Peng was supported by the
International Science & Technology Cooperation Program of China (Grant
Nos. 2013DFG52740 and 2010DFA52150) and the Natural Science Foundation
of China (Grant Nos. 51473053 and 51073060). T. P. Russell and F. Liu
were supported by the U.S. Office of Naval Research under contract
N00014-15-1-2244. Portions of this research were carried out at beamline
7.3.3 and 11.0.1.2 at the Advanced Light Source, and Molecular Foundry,
Lawrence Berkeley National Laboratory, which was supported by the DOE,
Office of Science, and Office of Basic Energy Sciences.
NR 41
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U1 92
U2 92
PU WILEY-V C H VERLAG GMBH
PI WEINHEIM
PA POSTFACH 101161, 69451 WEINHEIM, GERMANY
SN 0935-9648
EI 1521-4095
J9 ADV MATER
JI Adv. Mater.
PD OCT 5
PY 2016
VL 28
IS 37
BP 8184
EP 8190
DI 10.1002/adma.201602834
PG 7
WC Chemistry, Multidisciplinary; Chemistry, Physical; Nanoscience &
Nanotechnology; Materials Science, Multidisciplinary; Physics, Applied;
Physics, Condensed Matter
SC Chemistry; Science & Technology - Other Topics; Materials Science;
Physics
GA DZ8EL
UT WOS:000386103600011
PM 27414963
ER
PT J
AU Li, XF
Lin, MW
Basile, L
Hus, SM
Puretzky, AA
Lee, J
Kuo, YC
Chang, LY
Wang, K
Idrobo, JC
Li, AP
Chen, CH
Rouleau, CM
Geohegan, DB
Xiao, K
AF Li, Xufan
Lin, Ming-Wei
Basile, Leonardo
Hus, Saban M.
Puretzky, Alexander A.
Lee, Jaekwang
Kuo, Yen-Chien
Chang, Lo-Yueh
Wang, Kai
Idrobo, Juan C.
Li, An-Ping
Chen, Chia-Hao
Rouleau, Christopher M.
Geohegan, David B.
Xiao, Kai
TI Isoelectronic Tungsten Doping in Monolayer MoSe2 for Carrier Type
Modulation
SO ADVANCED MATERIALS
LA English
DT Article
DE alloys; carrier type modulation; isoelectronic; Mo1-xWxSe2; p-n
homojunctions
ID ELECTRONIC-PROPERTIES; MOLYBDENUM-DISULFIDE; SEMICONDUCTOR; GROWTH;
ALLOY; HETEROJUNCTION; SPECTROSCOPY; TRANSISTORS; ABSORPTION; DIODES
AB Carrier-type modulation is demonstrated in 2D transition metal dichalcogenides as n-type monolayer MoSe2 is converted to nondegenerate p-type monolayer Mo1-xWxSe2 through isoelectronic doping. Although the alloys are mesoscopically uniform, the p-type conduction in mono layer Mo1-xWxSe2 appears to originate from the upshift of the valence-band maximum toward the Fermi level at highly localized "W-rich" regions in the lattice.
C1 [Li, Xufan; Lin, Ming-Wei; Hus, Saban M.; Puretzky, Alexander A.; Wang, Kai; Idrobo, Juan C.; Li, An-Ping; Rouleau, Christopher M.; Geohegan, David B.; Xiao, Kai] Oak Ridge Natl Lab, Ctr Nanophase Mat Sci, Oak Ridge, TN 37831 USA.
[Basile, Leonardo] Escuela Politec Nacl, Dept Fis, Quito 17012759, Ecuador.
[Lee, Jaekwang] Pusan Natl Univ, Dept Phys, Busan 609735, South Korea.
[Kuo, Yen-Chien; Chang, Lo-Yueh; Chen, Chia-Hao] NSRRC, Hsinchu 30076, Taiwan.
RP Xiao, K (reprint author), Oak Ridge Natl Lab, Ctr Nanophase Mat Sci, Oak Ridge, TN 37831 USA.
EM xiaok@ornl.gov
RI Li, Xufan/A-8292-2013; Li, An-Ping/B-3191-2012
OI Li, Xufan/0000-0001-9814-0383; Li, An-Ping/0000-0003-4400-7493
FU Materials Science and Engineering Division, Office of Basic Energy
Sciences, U.S. Department of Energy
FX Special thanks goes to Mr. Ting Cao from Department of Physics at
University of California Berkeley, Dr. Bing Huang from Beijing
Computational Science Research Center, and Dr. Mina Yoon and Dr. Bobby
G. Sumpter from Center for Nanophase Materials Sciences at Oak Ridge
National Laboratory for their valuable discussion and advice on the
electronic structure of monolayer MoSe2 and
Mo1-xWxSe2. Synthesis science sponsored
by the Materials Science and Engineering Division, Office of Basic
Energy Sciences, U.S. Department of Energy. Materials characterization
was conducted at the Center for Nanophase Materials Sciences, which is a
DOE Office of Science User Facility.
NR 42
TC 3
Z9 3
U1 24
U2 24
PU WILEY-V C H VERLAG GMBH
PI WEINHEIM
PA POSTFACH 101161, 69451 WEINHEIM, GERMANY
SN 0935-9648
EI 1521-4095
J9 ADV MATER
JI Adv. Mater.
PD OCT 5
PY 2016
VL 28
IS 37
BP 8240
EP 8247
DI 10.1002/adma.201601991
PG 8
WC Chemistry, Multidisciplinary; Chemistry, Physical; Nanoscience &
Nanotechnology; Materials Science, Multidisciplinary; Physics, Applied;
Physics, Condensed Matter
SC Chemistry; Science & Technology - Other Topics; Materials Science;
Physics
GA DZ8EL
UT WOS:000386103600019
PM 27384240
ER
PT J
AU Li, B
Huang, L
Zhao, GY
Wei, ZM
Dong, HL
Hu, WP
Wang, LW
Li, JB
AF Li, Bo
Huang, Le
Zhao, Guangyao
Wei, Zhongming
Dong, Huanli
Hu, Wenping
Wang, Lin-Wang
Li, Jingbo
TI Large-Size 2D-Cu2S Nanosheets with Giant Phase Transition Temperature
Lowering (120 K) Synthesized by a Novel Method of Super-Cooling
Chemical-Vapor-Deposition
SO ADVANCED MATERIALS
LA English
DT Article
DE 2D materials; Cu2S; nanosheets; phase transition materials
ID COPPER SULFIDE; CU2S NANOCRYSTALS; NANOWIRE ARRAYS; SURFACE; GROWTH;
PRECURSORS; CHALCOCITE; NANODISKS; NANOSTRUCTURES; NONVOLATILE
AB 2D triangular beta-Cu2S nanosheets with large size and high quality are synthesized by a novel method of super-cooling chemical-vapor-deposition. The phase transition of this 2D material from beta-Cu2S to gamma-Cu2S occurs at 258 K (-15 degrees C), and such transition temperature is 120 K lower than that of its bulk counterpart (about 378 K).
C1 [Li, Bo; Huang, Le; Wei, Zhongming; Li, Jingbo] Chinese Acad Sci, State Key Lab Superlattices & Microstruct, Inst Semicond, Beijing 100083, Peoples R China.
[Zhao, Guangyao; Dong, Huanli; Hu, Wenping] Chinese Acad Sci, Beijing Natl Lab Mol Sci, Inst Chem, Key Lab Organ Solids, Beijing 100190, Peoples R China.
[Zhao, Guangyao] Global Energy Interconnect Res Inst, State Key Lab Adv Transmiss Technol, Future Sci & Technol Pk, Beijing 102211, Peoples R China.
[Hu, Wenping] Tianjin Univ, Tianjin Key Lab Mol Optoelect Sci, Dept Chem, Sch Sci, Tianjin 300072, Peoples R China.
[Hu, Wenping] Collaborat Innovat Ctr Chem Sci & Engn Tianjin, Tianjin 300072, Peoples R China.
[Wang, Lin-Wang] Lawrence Berkeley Natl Lab, Div Mat Sci, Berkeley, CA 94720 USA.
RP Wei, ZM; Li, JB (reprint author), Chinese Acad Sci, State Key Lab Superlattices & Microstruct, Inst Semicond, Beijing 100083, Peoples R China.; Hu, WP (reprint author), Chinese Acad Sci, Beijing Natl Lab Mol Sci, Inst Chem, Key Lab Organ Solids, Beijing 100190, Peoples R China.; Hu, WP (reprint author), Tianjin Univ, Tianjin Key Lab Mol Optoelect Sci, Dept Chem, Sch Sci, Tianjin 300072, Peoples R China.; Hu, WP (reprint author), Collaborat Innovat Ctr Chem Sci & Engn Tianjin, Tianjin 300072, Peoples R China.; Wang, LW (reprint author), Lawrence Berkeley Natl Lab, Div Mat Sci, Berkeley, CA 94720 USA.
EM zmwei@semi.ac.cn; huwp@iccas.ac.cn; lwwang@lbl.gov; jbli@semi.ac.cn
FU National Natural Science Foundation of China [61571415, 51502283,
61201105, 91027043, 91222203, 91233205, 91433115]; Ministry of Science
and Technology of China [2013CB933403, 2013CB933500]; Strategic Priority
Research Program of the Chinese Academy of Sciences (CAS) [XDB12030300];
"Hundred Talents Program" of Chinese Academy of Sciences; CAS/SAFEA
International Partnership Program for Creative Research Teams
FX The authors acknowledge National Natural Science Foundation of China
(61571415, 51502283, 61201105, 91027043, 91222203, 91233205, 91433115),
Ministry of Science and Technology of China (2013CB933403,
2013CB933500), the Strategic Priority Research Program of the Chinese
Academy of Sciences (CAS, XDB12030300). ZW acknowledges financial
support from the "Hundred Talents Program" of Chinese Academy of
Sciences. HD acknowledges Beijing Local College Innovation Team Improve
Plan (IDHT20140512). JL thankfully acknowledges financial support from
the CAS/SAFEA International Partnership Program for Creative Research
Teams.
NR 53
TC 1
Z9 1
U1 47
U2 47
PU WILEY-V C H VERLAG GMBH
PI WEINHEIM
PA POSTFACH 101161, 69451 WEINHEIM, GERMANY
SN 0935-9648
EI 1521-4095
J9 ADV MATER
JI Adv. Mater.
PD OCT 5
PY 2016
VL 28
IS 37
BP 8271
EP 8276
DI 10.1002/adma.201602701
PG 6
WC Chemistry, Multidisciplinary; Chemistry, Physical; Nanoscience &
Nanotechnology; Materials Science, Multidisciplinary; Physics, Applied;
Physics, Condensed Matter
SC Chemistry; Science & Technology - Other Topics; Materials Science;
Physics
GA DZ8EL
UT WOS:000386103600023
PM 27441730
ER
PT J
AU Gao, L
Zhang, ZG
Bin, HJ
Xue, LW
Yang, YK
Wang, C
Liu, F
Russell, TP
Li, YF
AF Gao, Liang
Zhang, Zhi-Guo
Bin, Haijun
Xue, Lingwei
Yang, Yankang
Wang, Cheng
Liu, Feng
Russell, Thomas P.
Li, Yongfang
TI High-Efficiency Nonfullerene Polymer Solar Cells with Medium Bandgap
Polymer Donor and Narrow Bandgap Organic Semiconductor Acceptor
SO ADVANCED MATERIALS
LA English
DT Article
DE extinction coefficients; fluorinated conjugated polymer donors; ITIC;
nonfullerene polymer solar cells
ID POWER CONVERSION EFFICIENCY; NON-FULLERENE ACCEPTOR; SMALL-MOLECULE
ACCEPTOR; OPEN-CIRCUIT VOLTAGE; CATHODE INTERLAYER; ELECTRON-ACCEPTORS;
PHASE-SEPARATION; PHOTOVOLTAICS; ABSORPTION; DIKETOPYRROLOPYRROLE
AB A nonfullerene polymer solar cell with a high efficiency of 9.26% is realized by using benzodithiophene-alt-fluorobenzotriazole copolymer J51 as a medium-bandgap polymer donor and the low-bandgap organic semiconductor ITIC with high extinction coefficients as the acceptor.
C1 [Gao, Liang; Zhang, Zhi-Guo; Bin, Haijun; Xue, Lingwei; Yang, Yankang; Li, Yongfang] Chinese Acad Sci, Beijing Natl Lab Mol Sci, CAS Key Lab Organ Solids, Inst Chem, Beijing 100190, Peoples R China.
[Gao, Liang; Bin, Haijun; Yang, Yankang; Li, Yongfang] Univ Chinese Acad Sci, Beijing 100049, Peoples R China.
[Wang, Cheng] Lawrence Berkeley Natl Lab, Adv Light Source, Berkeley, CA 94720 USA.
[Liu, Feng] Lawrence Berkeley Natl Lab, Div Mat Sci, Berkeley, CA 94720 USA.
[Russell, Thomas P.] Univ Massachusetts, Polymer Sci & Engn Dept, Amherst, MA 01003 USA.
[Li, Yongfang] Soochow Univ, Lab Adv Optoelect Mat, Coll Chem Chem Engn & Mat Sci, Suzhou 215123, Jiangsu, Peoples R China.
RP Zhang, ZG; Li, YF (reprint author), Chinese Acad Sci, Beijing Natl Lab Mol Sci, CAS Key Lab Organ Solids, Inst Chem, Beijing 100190, Peoples R China.; Li, YF (reprint author), Univ Chinese Acad Sci, Beijing 100049, Peoples R China.; Liu, F (reprint author), Lawrence Berkeley Natl Lab, Div Mat Sci, Berkeley, CA 94720 USA.; Li, YF (reprint author), Soochow Univ, Lab Adv Optoelect Mat, Coll Chem Chem Engn & Mat Sci, Suzhou 215123, Jiangsu, Peoples R China.
EM zgzhangwhu@iccas.ac.cn; iamfengliu@gmail.com; liyf@iccas.ac.cn
RI Wang, Cheng/A-9815-2014; Liu, Feng/J-4361-2014
OI Liu, Feng/0000-0002-5572-8512
FU Ministry of Science and Technology of China (973 project)
[2014CB643501]; NSFC [91433117, 91333204, 21374124]; Strategic Priority
Research Program of the Chinese Academy of Sciences [XDB12030200]; U.S.
Office of Naval Research [N00014-15-1-2244]; DOE, Office of Science, and
Office of Basic Energy Sciences
FX The work was supported by the Ministry of Science and Technology of
China (973 project, No. 2014CB643501) and NSFC (Nos. 91433117, 91333204,
and 21374124) and the Strategic Priority Research Program of the Chinese
Academy of Sciences, Grant No. XDB12030200. F.L. and T.P.R. were
supported by the U.S. Office of Naval Research under contract
N00014-15-1-2244. Portions of this research were carried out at beamline
7.3.3 and 11.0.1.2 at the Advanced Light Source, and Molecular Foundry,
Lawrence Berkeley National Laboratory, which was supported by the DOE,
Office of Science, and Office of Basic Energy Sciences.
NR 56
TC 9
Z9 9
U1 120
U2 120
PU WILEY-V C H VERLAG GMBH
PI WEINHEIM
PA POSTFACH 101161, 69451 WEINHEIM, GERMANY
SN 0935-9648
EI 1521-4095
J9 ADV MATER
JI Adv. Mater.
PD OCT 5
PY 2016
VL 28
IS 37
BP 8288
EP 8295
DI 10.1002/adma.201601595
PG 8
WC Chemistry, Multidisciplinary; Chemistry, Physical; Nanoscience &
Nanotechnology; Materials Science, Multidisciplinary; Physics, Applied;
Physics, Condensed Matter
SC Chemistry; Science & Technology - Other Topics; Materials Science;
Physics
GA DZ8EL
UT WOS:000386103600026
PM 27386802
ER
PT J
AU Chakraborty, A
Tapryal, N
Venkova, T
Horikoshi, N
Pandita, RK
Sarker, AH
Sarkar, PS
Pandita, TK
Hazra, TK
AF Chakraborty, Anirban
Tapryal, Nisha
Venkova, Tatiana
Horikoshi, Nobuo
Pandita, Raj K.
Sarker, Altaf H.
Sarkar, Partha S.
Pandita, Tej K.
Hazra, Tapas K.
TI Classical non-homologous end-joining pathway utilizes nascent RNA for
error-free double-strand break repair of transcribed genes
SO NATURE COMMUNICATIONS
LA English
DT Article
ID POLYNUCLEOTIDE KINASE 3'-PHOSPHATASE; DNA-DAMAGE RESPONSE; HOMOLOGOUS
RECOMBINATION; HUMAN-CELLS; POLYMERASE-II; PROTEIN; GENOME; EXPRESSION;
TRANSLOCATIONS; RECOGNITION
AB DNA double-strand breaks (DSBs) leading to loss of nucleotides in the transcribed region can be lethal. Classical non-homologous end-joining (C-NHEJ) is the dominant pathway for DSB repair (DSBR) in adult mammalian cells. Here we report that during such DSBR, mammalian C-NHEJ proteins form a multiprotein complex with RNA polymerase II and preferentially associate with the transcribed genes after DSB induction. Depletion of C-NHEJ factors significantly abrogates DSBR in transcribed but not in non-transcribed genes. We hypothesized that nascent RNA can serve as a template for restoring the missing sequences, thus allowing error-free DSBR. We indeed found pre-mRNA in the C-NHEJ complex. Finally, when a DSB-containing plasmid with several nucleotides deleted within the E. coli lacZ gene was allowed time to repair in lacZ-expressing mammalian cells, a functional lacZ plasmid could be recovered from control but not C-NHEJ factor-depleted cells, providing important mechanistic insights into C-NHEJ-mediated error-free DSBR of the transcribed genome.
C1 [Chakraborty, Anirban; Tapryal, Nisha; Venkova, Tatiana; Hazra, Tapas K.] Univ Texas Med Branch, Dept Internal Med, Sealy Ctr Mol Med, Div Pulm & Crit Care Med, Galveston, TX 77555 USA.
[Horikoshi, Nobuo; Pandita, Raj K.; Pandita, Tej K.] Houston Methodist Res Inst, Dept Radiat Oncol, Houston, TX 77030 USA.
[Sarker, Altaf H.] Lawrence Berkeley Natl Lab, Dept Canc & DNA Damage Responses, Div Life Sci, Berkeley, CA 94720 USA.
[Sarkar, Partha S.] Univ Texas Med Branch, Dept Neurol & Neurosci & Cell Biol, Galveston, TX 77555 USA.
RP Hazra, TK (reprint author), Univ Texas Med Branch, Dept Internal Med, Sealy Ctr Mol Med, Div Pulm & Crit Care Med, Galveston, TX 77555 USA.
EM tkhazra@utmb.edu
FU National Institute of Health from the USPHS [R01 NS073976, R01 NS096305,
R01 CA129537, R01 GM109768, P01 AI062885]; [P30 ES 06676]
FX This work was supported, in whole or in part, by National Institute of
Health Grants R01 NS073976 (to T.K.H.) and R01 NS096305 (to P.S.S. and
T.K.H.), and R01 CA129537 and R01 GM109768 (to T.K.P.) and P01 AI062885
(to I.B.) from the USPHS, and Grant P30 ES 06676 to the NIEHS Center
Cell Biology Core and Molecular Genomics Core of UTMB's NIEHS Center for
DNA Sequencing. We thank Dr David Konkel for critically editing this
manuscript, Justin Barr of IDT for designing LA-qPCR primers for NANOG
and OCT3/4 human genes, and Dr Bradford D Loucas of Radiation Oncology,
UTMB for his generous help in performing IR exposure.
NR 50
TC 2
Z9 2
U1 5
U2 5
PU NATURE PUBLISHING GROUP
PI LONDON
PA MACMILLAN BUILDING, 4 CRINAN ST, LONDON N1 9XW, ENGLAND
SN 2041-1723
J9 NAT COMMUN
JI Nat. Commun.
PD OCT 5
PY 2016
VL 7
AR 13049
DI 10.1038/ncomms13049
PG 12
WC Multidisciplinary Sciences
SC Science & Technology - Other Topics
GA DZ0SW
UT WOS:000385551000001
PM 27703167
ER
PT J
AU Dickel, DE
Barozzi, I
Zhu, YW
Fukuda-Yuzawa, Y
Osterwalder, M
Mannion, BJ
May, D
Spurrell, CH
Plajzer-Frick, I
Pickle, CS
Lee, E
Garvin, TH
Kato, M
Akiyama, JA
Afzal, V
Lee, AY
Gorkin, DU
Ren, B
Rubin, EM
Visel, A
Pennacchio, LA
AF Dickel, Diane E.
Barozzi, Iros
Zhu, Yiwen
Fukuda-Yuzawa, Yoko
Osterwalder, Marco
Mannion, Brandon J.
May, Dalit
Spurrell, Cailyn H.
Plajzer-Frick, Ingrid
Pickle, Catherine S.
Lee, Elizabeth
Garvin, Tyler H.
Kato, Momoe
Akiyama, Jennifer A.
Afzal, Veena
Lee, Ah Young
Gorkin, David U.
Ren, Bing
Rubin, Edward M.
Visel, Axel
Pennacchio, Len A.
TI Genome-wide compendium and functional assessment of in vivo heart
enhancers
SO NATURE COMMUNICATIONS
LA English
DT Article
ID GENE-EXPRESSION; TRANSCRIPTION FACTORS; MOUSE GENOME; HISTONE
MODIFICATIONS; REGULATORY ELEMENTS; SUSCEPTIBILITY LOCI; EMBRYONIC LIMB;
RNA-SEQ; DISEASE; IDENTIFICATION
AB Whole-genome sequencing is identifying growing numbers of non-coding variants in human disease studies, but the lack of accurate functional annotations prevents their interpretation. We describe the genome-wide landscape of distant-acting enhancers active in the developing and adult human heart, an organ whose impairment is a predominant cause of mortality and morbidity. Using integrative analysis of >35 epigenomic data sets from mouse and human pre- and postnatal hearts we created a comprehensive reference of >80,000 putative human heart enhancers. To illustrate the importance of enhancers in the regulation of genes involved in heart disease, we deleted the mouse orthologs of two human enhancers near cardiac myosin genes. In both cases, we observe in vivo expression changes and cardiac phenotypes consistent with human heart disease. Our study provides a comprehensive catalogue of human heart enhancers for use in clinical whole-genome sequencing studies and highlights the importance of enhancers for cardiac function.
C1 [Dickel, Diane E.; Barozzi, Iros; Zhu, Yiwen; Fukuda-Yuzawa, Yoko; Osterwalder, Marco; Mannion, Brandon J.; May, Dalit; Spurrell, Cailyn H.; Plajzer-Frick, Ingrid; Pickle, Catherine S.; Lee, Elizabeth; Garvin, Tyler H.; Kato, Momoe; Akiyama, Jennifer A.; Afzal, Veena; Rubin, Edward M.; Visel, Axel; Pennacchio, Len A.] Lawrence Berkeley Natl Lab, Funct Genom Dept, 1 Cyclotron Rd, Berkeley, CA 94720 USA.
[Lee, Ah Young; Gorkin, David U.; Ren, Bing] Ludwig Inst Canc Res, 9500 Gilman Dr, La Jolla, CA 92093 USA.
[Ren, Bing] Univ Calif San Diego, Sch Med, Dept Cellular & Mol Med, La Jolla, CA 92093 USA.
[Rubin, Edward M.; Visel, Axel; Pennacchio, Len A.] US DOE, Joint Genome Inst, Walnut Creek, CA 94598 USA.
[Visel, Axel] Univ Calif Merced, Sch Nat Sci, Merced, CA 95343 USA.
[May, Dalit] Hebrew Univ Jerusalem, Hadassah Med Sch, Dept Family Med, Clalit Hlth Serv, IL-91120 Jerusalem, Israel.
RP Dickel, DE; Visel, A; Pennacchio, LA (reprint author), Lawrence Berkeley Natl Lab, Funct Genom Dept, 1 Cyclotron Rd, Berkeley, CA 94720 USA.; Visel, A; Pennacchio, LA (reprint author), US DOE, Joint Genome Inst, Walnut Creek, CA 94598 USA.; Visel, A (reprint author), Univ Calif Merced, Sch Nat Sci, Merced, CA 95343 USA.
EM dedickel@lbl.gov; avisel@lbl.gov; lapennacchio@lbl.gov
RI Visel, Axel/A-9398-2009;
OI Visel, Axel/0000-0002-4130-7784; Dickel, Diane/0000-0001-5497-6824
FU National Institutes of Health [R24HL123879, U01DE024427, R01HG003988,
U54HG006997, UM1HL098166]; Swiss National Science Foundation (SNSF)
fellowship; Department of Energy [DE-AC02-05CH11231]; National Institute
of Health [S10RR029668, S10RR027303]; National Institute of Diabetes and
Digestive and Kidney Diseases [U24DK092993]
FX This work was supported by National Institutes of Health grants
R24HL123879, U01DE024427, R01HG003988, U54HG006997 and UM1HL098166. M.O.
was supported by a Swiss National Science Foundation (SNSF) fellowship.
Research was conducted at the E.O. Lawrence Berkeley National Laboratory
and performed under Department of Energy Contract DE-AC02-05CH11231,
University of California. This work used the Vincent J. Coates Genomics
Sequencing Laboratory at UC Berkeley, which is supported by National
Institute of Health Grants S10RR029668 and S10RR027303. Histology,
pathology and echocardiography were performed at the University of
California Davis Mouse Metabolic Phenotyping Center, which is supported
by National Institute of Diabetes and Digestive and Kidney Diseases
grant U24DK092993. We would like to thank N. Chiamvimonvat (University
of California Davis) for help in performing and interpreting the
echocardiography testing.
NR 73
TC 3
Z9 3
U1 2
U2 2
PU NATURE PUBLISHING GROUP
PI LONDON
PA MACMILLAN BUILDING, 4 CRINAN ST, LONDON N1 9XW, ENGLAND
SN 2041-1723
J9 NAT COMMUN
JI Nat. Commun.
PD OCT 5
PY 2016
VL 7
AR 12923
DI 10.1038/ncomms12923
PG 13
WC Multidisciplinary Sciences
SC Science & Technology - Other Topics
GA DZ0QD
UT WOS:000385543900001
PM 27703156
ER
PT J
AU Wei, T
Chen, TC
Ho, YT
Ronald, PC
AF Wei, Tong
Chen, Tsung-Chi
Ho, Yuen Ting
Ronald, Pamela C.
TI Mutation of the rice 21 predicted nuclear localization sequence does not
affect resistance to Xanthomonas oryzae pv. oryzae
SO PEERJ
LA English
DT Article
DE Nuclear localization; Bacterial blight disease; Xanthomonas oryzae pv.
oryzae; XA21-mediated immunity
ID CONSERVED MICROBIAL SIGNATURES; XA21-MEDIATED INNATE IMMUNITY;
PATTERN-RECOGNITION RECEPTOR; DISEASE RESISTANCE; XA21; PROTEIN;
AUTOPHOSPHORYLATION; PLANT
AB Background. The rice receptor kinase XA21 confers robust resistance to the bacterial pathogen Xanrhomonas oryzae pv. oryzae(Xoo). We previously reported that XA21 is cleaved in transgenic plants overexpressing XA21 with a GFP tag (Ubi-XA21-GFP) and that the released C-terminal domain is localized to the nucleus. XA21 carries a predicted nuclear localization sequence (NLS) that directs the C-terminal domain to the nucleus in transient assays, whereas alanine substitutions in the NLS disrupt the nuclear localization.
Methods. To determine if the predicted NLS is required for XA21-mediated immunity in planta we generated transgenic plants overexpressing an XA21 variant carrying the NLS with the same alanine substitutions (Ubi-XA21nls-GFP).
Results. Ubi-XA21nls-GFP plants displayed slightly longer lesion lengths, higher Xoo bacterial populations after inoculation and lower levels of reactive oxygen species production compared with the Ubi-XA21-GFP control plants. However, the Ubi-XA21-nls-GFP plants express lower levels of protein than that observed in Ubt-XA21-GFP.
Discussion. These results demonstrate that the predicted NLS is not required for XA21-mediated immunity.
C1 [Wei, Tong; Chen, Tsung-Chi; Ho, Yuen Ting; Ronald, Pamela C.] Univ Calif Davis, Dept Plant Pathol, Davis, CA 95616 USA.
[Wei, Tong; Chen, Tsung-Chi; Ho, Yuen Ting; Ronald, Pamela C.] Univ Calif Davis, Genome Ctr, Davis, CA 95616 USA.
[Wei, Tong; Ronald, Pamela C.] Lawrence Berkeley Natl Lab, Joint BioEnergy Inst, Feedstocks Div, Berkeley, CA 94720 USA.
[Wei, Tong; Ronald, Pamela C.] Lawrence Berkeley Natl Lab, Biol Syst & Engn Div, Berkeley, CA 94720 USA.
RP Ronald, PC (reprint author), Univ Calif Davis, Dept Plant Pathol, Davis, CA 95616 USA.; Ronald, PC (reprint author), Univ Calif Davis, Genome Ctr, Davis, CA 95616 USA.; Ronald, PC (reprint author), Lawrence Berkeley Natl Lab, Joint BioEnergy Inst, Feedstocks Div, Berkeley, CA 94720 USA.; Ronald, PC (reprint author), Lawrence Berkeley Natl Lab, Biol Syst & Engn Div, Berkeley, CA 94720 USA.
EM peronald@ucdavis.edu
FU NIH [GM59962]; Office of Science, Office of Biological and Environmental
Research of the US Department of Energy [DE-AC02-05CH11231]
FX The work was supported by NIH GM59962 to Pamela C. Ronald. The work
conducted by the Joint BioEnergy Institute was supported by the Office
of Science, Office of Biological and Environmental Research, of the US
Department of Energy under Contract No. DE-AC02-05CH11231. The funders
had no role in study design, data collection and analysis, decision to
publish, or preparation of the manuscript.
NR 15
TC 0
Z9 0
U1 1
U2 1
PU PEERJ INC
PI LONDON
PA 341-345 OLD ST, THIRD FLR, LONDON, EC1V 9LL, ENGLAND
SN 2167-8359
J9 PEERJ
JI PeerJ
PD OCT 5
PY 2016
VL 4
AR e2507
DI 10.7717/peerj.2507
PG 10
WC Multidisciplinary Sciences
SC Science & Technology - Other Topics
GA DZ1CV
UT WOS:000385577400004
PM 27761320
ER
PT J
AU Sushruth, M
Ding, JJ
Duczynski, J
Woodward, RC
Begley, RA
Fangohr, H
Fuller, RO
Adeyeye, AO
Kostylev, M
Metaxas, PJ
AF Sushruth, Manu
Ding, Junjia
Duczynski, Jeremy
Woodward, Robert C.
Begley, Ryan A.
Fangohr, Hans
Fuller, Rebecca O.
Adeyeye, Adekunle O.
Kostylev, Mikhail
Metaxas, Peter J.
TI Resonance-Based Detection of Magnetic Nanoparticles and Microbeads Using
Nanopatterned Ferromagnets
SO PHYSICAL REVIEW APPLIED
LA English
DT Article
ID FLOW-CYTOMETRY; BIOSENSOR; QUANTIFICATION; SENSOR; SENSITIVITY;
MEDICINE; SYSTEM; ASSAY
AB Biosensing with ferromagnet-based magnetoresistive devices has been dominated by electrical detection of particle-induced changes to a device's (quasi-) static magnetic configuration. There are however potential advantages to be gained from using field dependent, high frequency resonant magnetization dynamics for magnetic particle detection. Here, we demonstrate the use of nanoconfined ferromagnetic resonances in periodically nanopatterned magnetic films for the detection of adsorbed magnetic particles having diameters ranging from 6 nm to 4 mu m. The nanopatterned films contain arrays of holes which appear to act as preferential adsorption sites for small particles. Hole-localized particles act in unison to shift the frequencies of the patterned layer's ferromagnetic-resonance modes, with shift polarities determined by the localization of each mode within the nanopattern's repeating unit cell. The same polarity shifts are observed for a large range of coverages, even when quasicontinuous particle sheets form above the hole-localized particles. For large particles, preferential adsorption no longer occurs, leading to resonance shifts with polarities that are independent of the mode localization, and amplitudes that are comparable to those seen in continuous layers. Indeed, for nanoparticles adsorbed onto a continuous layer, the particle-induced shift of the layer's fundamental mode is up to 10 times less than that observed for nanoconfined modes in the nanopatterned systems, the low shift being induced by relatively weak fields emanating beyond the particle in the direction of the static applied field. This result highlights the importance of having particles consistently positioned in the close vicinity of confined modes.
C1 [Sushruth, Manu; Woodward, Robert C.; Begley, Ryan A.; Kostylev, Mikhail; Metaxas, Peter J.] Univ Western Australia, Sch Phys, M013,35 Stirling Highway, Crawley, WA 6009, Australia.
[Ding, Junjia; Adeyeye, Adekunle O.] Natl Univ Singapore, Dept Elect & Comp Engn, 4 Engn Dr 3, Singapore 117576, Singapore.
[Duczynski, Jeremy; Fuller, Rebecca O.] Univ Western Australia, Sch Chem & Biochem, M310,35 Stirling Highway, Crawley, WA 6009, Australia.
[Fangohr, Hans] Univ Southampton, Fac Engn & Environm, Southampton SO17 1BJ, Hants, England.
[Ding, Junjia] Argonne Natl Lab, 9700 South Cass Ave, Argonne, IL 60439 USA.
RP Metaxas, PJ (reprint author), Univ Western Australia, Sch Phys, M013,35 Stirling Highway, Crawley, WA 6009, Australia.
EM peter.metaxas@uwa.edu.au
RI Fangohr, Hans/C-6367-2008; DING, Junjia/K-2277-2013
OI Fangohr, Hans/0000-0001-5494-7193; DING, Junjia/0000-0002-9917-9156
FU Australian Research Council's Discovery Early Career Researcher Award
scheme [DE120100155]; Discovery Projects scheme [DP110103980]; U.S. Air
Force [Asian Office of Aerospace Research and Development (AOARD)];
Research Development Award; Research Collaboration Award; Early Career
Researcher Fellowship; International Research Fees; University
Postgraduate; Re-Entry Fellowship; Teaching Relief and School of Physics
Vacation Scholarship; Pawsey Supercomputing Centre; Australian
Government; Government of Western Australia; National Research
Foundation; Prime Minister's Office, Singapore [NRF-CRP10-201203];
University, State, and Commonwealth Governments
FX This research is supported by the Australian Research Council's
Discovery Early Career Researcher Award scheme (Grant No. DE120100155)
and Discovery Projects scheme (Grant No. DP110103980) and the U.S. Air
Force [Asian Office of Aerospace Research and Development (AOARD)]. The
University of Western Australia (UWA) also supported this research via
the following programs: Research Development Award, Research
Collaboration Award, Early Career Researcher Fellowship Support,
Scholarship for International Research Fees, University Postgraduate
Award (International Students), Re-Entry Fellowship, Teaching Relief and
School of Physics Vacation Scholarship. This work is also supported by
resources provided by the Pawsey Supercomputing Centre with funding from
the Australian Government and the Government of Western Australia.
A.O.A. is supported by the National Research Foundation, Prime
Minister's Office, Singapore under its Competitive Research Programme
(CRP Grant No. NRF-CRP10-201203). The authors thank C. Lueng, M. Albert,
W. Wang, A. Suvorova, A. Dodd, C. Yang, D. Schibeci, A. Chew, and R. C.
Bording for their assistance. The authors acknowledge access to the UWA
Biomagnetics Wet Laboratory and Magnetic Characterisation Facility and
the facilities and the scientific and technical assistance of the
Australian Microscopy & Microanalysis Research Facility at the Centre
for Microscopy, Characterisation and Analysis, The University of Western
Australia, a facility funded by the University, State, and Commonwealth
Governments.
NR 58
TC 0
Z9 0
U1 15
U2 15
PU AMER PHYSICAL SOC
PI COLLEGE PK
PA ONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA
SN 2331-7019
J9 PHYS REV APPL
JI Phys. Rev. Appl.
PD OCT 5
PY 2016
VL 6
IS 4
DI 10.1103/PhysRevApplied.6.044005
PG 12
WC Physics, Applied
SC Physics
GA DY7XL
UT WOS:000385342500001
ER
PT J
AU Hattori, K
Yin, Y
AF Hattori, Koichi
Yin, Yi
TI Charge Redistribution from Anomalous Magnetovorticity Coupling
SO PHYSICAL REVIEW LETTERS
LA English
DT Article
ID HEAVY-ION COLLISIONS; FINITE-TEMPERATURE; MAGNETIC-FIELD; EQUILIBRIUM;
VIOLATION; TRANSPORT; FERMIONS; SPIN
AB We investigate novel transport phenomena in a chiral fluid originated from an interplay between a vorticity and strong magnetic field, which induces a redistribution of vector charges in the system and an axial current along the magnetic field. The corresponding transport coefficients are obtained from an energy-shift argument for the chiral fermions in the lowest Landau level due to a spin-vorticity coupling and also from diagrammatic computations on the basis of the linear response theory. Based on consistent results from both methods, we observe that the transport coefficients are proportional to the anomaly coefficient and are independent of temperature and chemical potential. We therefore speculate that these transport phenomena are connected to quantum anomaly.
C1 [Hattori, Koichi] Fudan Univ, Dept Phys, Shanghai 200433, Peoples R China.
[Hattori, Koichi] Brookhaven Natl Lab, RIKEN BNL Res Ctr, Upton, NY 11973 USA.
[Yin, Yi] Brookhaven Natl Lab, Dept Phys, Upton, NY 11973 USA.
RP Hattori, K (reprint author), Fudan Univ, Dept Phys, Shanghai 200433, Peoples R China.; Hattori, K (reprint author), Brookhaven Natl Lab, RIKEN BNL Res Ctr, Upton, NY 11973 USA.
FU China Postdoctoral Science Foundation [2016M590312]; Japan Society for
the Promotion of Science [25287066]; RIKEN-BNL Research Center; U.S.
Department of Energy, Office of Science, Office of Nuclear Physics
[DE-SC0012704]
FX We would like to thank Y. Hidaka, Y. Hirono, M. Hongo, D. Kharzeev, L.
McLerran, R. Pisarski, P. Surowka, M. Stephanov, and H.-U. Yee for
helpful discussions, and K. Fukushima, X.-G. Huang, S. Lin, D. Satow,
and N. Yamamoto for comments on the draft. Y. Y. also acknowledges the
stimulating environment of the "QCD Chirality" workshop at UCLA. This
work is supported in part by China Postdoctoral Science Foundation under
Grant No. 2016M590312 and, at the early stage, by Japan Society for the
Promotion of Science Grants-in-Aid No. 25287066 (K. H.). K. H. is also
grateful for support from RIKEN-BNL Research Center. This material is
based upon work supported in part by the U.S. Department of Energy,
Office of Science, Office of Nuclear Physics, under Contract No.
DE-SC0012704, and within the framework of the Beam Energy Scan Theory
(BEST) Topical Collaboration (Y. Y.).
NR 35
TC 0
Z9 0
U1 3
U2 3
PU AMER PHYSICAL SOC
PI COLLEGE PK
PA ONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA
SN 0031-9007
EI 1079-7114
J9 PHYS REV LETT
JI Phys. Rev. Lett.
PD OCT 5
PY 2016
VL 117
IS 15
AR 152002
DI 10.1103/PhysRevLett.117.152002
PG 5
WC Physics, Multidisciplinary
SC Physics
GA DY7XC
UT WOS:000385341600002
PM 27768344
ER
PT J
AU Peterman, D
Geist, A
Mincher, B
Modolo, G
Galan, MH
Olson, L
McDowell, R
AF Peterman, Dean
Geist, Andreas
Mincher, Bruce
Modolo, Giuseppe
Galan, Maria Hitos
Olson, Lonnie
McDowell, Rocklan
TI Performance of an i-SANEX System Based on a Water-Soluble BTP under
Continuous Irradiation in a gamma-Radiolysis Test Loop
SO INDUSTRIAL & ENGINEERING CHEMISTRY RESEARCH
LA English
DT Article
ID SOLVENT-EXTRACTION; PUREX RAFFINATE; NITRIC-ACID; TODGA; STABILITY;
SEPARATION; ACTINIDES; RADIATION; COMPLEXATION; MIXTURES
AB The i-SANEX solvent formulation consisting of nominally 0.2 M TODGA/5% 1-octanol/dodecane was gamma-irradiated under realistic conditions in the Idaho National Laboratory radiolysis test loop, in contact with both extraction and stripping aqueous phases. The extraction aqueous phase was 4.5 M HNO3, and the stripping aqueous phase was 0.018 M SO3-Ph-BTP/0.35 M HNO3. When irradiated in contact with only the 4.5 M HNO3 phase, the TODGA solvent maintained excellent extraction performance for americium, cerium, europium, and neodymium to a maximum absorbed dose of nearly 0.9 MGy. The results for preliminary static, batch irradiations were consistent with test loop findings. When the aqueous phase was changed to that containing the aqueous soluble BTP, the irradiated aqueous phase showed a dramatic color change, but this does not appear to have had adverse effect on solvent extraction performance. The distribution ratios for both the lanthanides and actinides were invariant with absorbed dose, and the separation factors were essentially unchanged to a maximum absorbed dose of 174 kGy. The results of inductively coupled plasma mass spectrometry analysis of the aqueous and organic phases showed that ruthenium and strontium were not extracted in the presence of the irradiated BTP-aqueous phase. Molybdenum was extracted under both conditions. Further, the buildup of corrosion products of stainless steel in the presence of the BTP was not dramatically greater than in the nitric acid-only system. Phase separation times were not adversely affected by irradiation for either system. The results presented here indicate that the performance of the TODGA/SO3-Ph BTP, i-SANEX process under test loop radiolysis is much better than expected based on a literature report using single-phase batch irradiation experiments, and better than might be predicted based on diglycolamide radiolysis studies alone.
C1 [Peterman, Dean; Mincher, Bruce; Olson, Lonnie; McDowell, Rocklan] Idaho Natl Lab, Aqueous Separat & Radiochem Dept, Idaho Falls, ID 83415 USA.
[Geist, Andreas] Karlsruhe Inst Technol, Inst Nucl Waste Disposal INE, POB 3640, D-76021 Karlsruhe, Germany.
[Modolo, Giuseppe] Forschungszentrum Julich, Inst Energy & Climate Res, Nucl Waste Management & Reactor Safety IEK 6, D-52425 Julich, Germany.
[Galan, Maria Hitos] Ctr Invest Energet Medioambientales & Tecnol CIEM, Madrid 28040, Spain.
RP Peterman, D (reprint author), Idaho Natl Lab, Aqueous Separat & Radiochem Dept, Idaho Falls, ID 83415 USA.
EM dean.peterman@inl.gov
RI Mincher, Bruce/C-7758-2017
FU U.S. Department of Energy, Office of Nuclear Energy, through the Fuel
Cycle Research and Development Program; Battelle Energy Alliance under
DOE Idaho Operations Office [DE-AC07-05ID14517]
FX This research was sponsored by the U.S. Department of Energy, Office of
Nuclear Energy, through the Fuel Cycle Research and Development Program.
Idaho National Laboratory is operated by Battelle Energy Alliance under
DOE Idaho Operations Office Contract DE-AC07-05ID14517.
NR 27
TC 1
Z9 1
U1 6
U2 6
PU AMER CHEMICAL SOC
PI WASHINGTON
PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA
SN 0888-5885
J9 IND ENG CHEM RES
JI Ind. Eng. Chem. Res.
PD OCT 5
PY 2016
VL 55
IS 39
BP 10427
EP 10435
DI 10.1021/acs.iecr.6b02862
PG 9
WC Engineering, Chemical
SC Engineering
GA DY2WH
UT WOS:000384952300022
ER
PT J
AU Lu, LQ
Yoo, K
Benyahia, S
AF Lu, Liqiang
Yoo, Kisoo
Benyahia, Sofiane
TI Coarse-Grained-Particle Method for Simulation of Liquid-Solids Reacting
Flows
SO INDUSTRIAL & ENGINEERING CHEMISTRY RESEARCH
LA English
DT Article
ID FLUIDIZED-BED; DEM SIMULATIONS; CFD SIMULATION; GAS; MODEL
AB A coarse-grained-particle method (CGPM) that tracks fewer particles and their collisions by lumping several real particles into computational parcels is developed. We demonstrate that the accuracy of CGPM can be improved by properly selecting interpolation schemes used to compute flow variables at particle and computational grid locations. The computational speed of CGPM was shown to be similar to that of a widely used and less accurate particle in cell method (PIC). Finally, a chemical reaction mechanism based on rare earth elements (REE) leaching from coal byproducts was implemented with CGPM to study the effects of several flow and design parameters on the leaching process. A countercurrent reactor was studied and optimized to maximize the mass fraction of REE in the liquid solution. The CGPM can now be employed to cheaply and accurately solve industrial-scale problems containing millions of computational parcels.
C1 [Lu, Liqiang; Yoo, Kisoo; Benyahia, Sofiane] Natl Energy Technol Lab, Morgantown, WV 26507 USA.
RP Benyahia, S (reprint author), Natl Energy Technol Lab, Morgantown, WV 26507 USA.
EM sofiane.benyahia@netl.doe.gov
OI Lu, Liqiang/0000-0002-5101-1688
FU U.S. Department of Energy
FX This research was supported in part by an appointment to the National
Energy Technology Laboratory Research Participation Program, sponsored
by the U.S. Department of Energy and administered by the Oak Ridge
Institute for Science and Education.
NR 41
TC 0
Z9 0
U1 17
U2 17
PU AMER CHEMICAL SOC
PI WASHINGTON
PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA
SN 0888-5885
J9 IND ENG CHEM RES
JI Ind. Eng. Chem. Res.
PD OCT 5
PY 2016
VL 55
IS 39
BP 10477
EP 10491
DI 10.1021/acs.iecr.6b02688
PG 15
WC Engineering, Chemical
SC Engineering
GA DY2WH
UT WOS:000384952300027
ER
PT J
AU Singh, MR
Kwon, Y
Lum, Y
Ager, JW
Bell, AT
AF Singh, Meenesh R.
Kwon, Youngkook
Lum, Yanwei
Ager, Joel W., III
Bell, Alexis T.
TI Hydrolysis of Electrolyte Cations Enhances the Electrochemical Reduction
of CO2 over Ag and Cu
SO JOURNAL OF THE AMERICAN CHEMICAL SOCIETY
LA English
DT Article
ID CARBON-DIOXIDE; MERCURY-ELECTRODE; AQUEOUS-SOLUTION; PRODUCT; COPPER;
ELECTROREDUCTION; ADSORPTION; FUTURE; ENERGY; FUELS
AB Electrolyte cation size is known to influence the electrochemical reduction of CO2 over metals; however, a satisfactory explanation for this phenomenon has not been developed. We report here that these effects can be attributed to a previously unrecognized consequence of cation hydrolysis occurring in the vicinity of the cathode. With increasing cation size, the pKa for cation hydrolysis decreases and is sufficiently low for hydrated K+, Rb+, and Cs+ to serve as buffering agents. Buffering lowers the pH near the cathode, leading to an increase in the local concentration of dissolved CO2. The consequences of these changes are an increase in cathode activity, a decrease in Faradaic efficiencies for H-2 and CH4, and an increase in Faradaic efficiencies for CO, C2H4, and C2H5OH, in full agreement with experimental observations for CO2 reduction over Ag and Cu.
C1 [Kwon, Youngkook] Korea Res Inst Chem Technol, Carbon Resources Inst, Daejeon 34114, South Korea.
[Singh, Meenesh R.; Kwon, Youngkook; Lum, Yanwei; Ager, Joel W., III; Bell, Alexis T.] Lawrence Berkeley Natl Lab, Div Mat Sci, Joint Ctr Artificial Photosynth, Berkeley, CA 94720 USA.
[Singh, Meenesh R.] Univ Illinois, Dept Chem Engn, Chicago, IL 60607 USA.
[Bell, Alexis T.] Univ Calif Berkeley, Dept Chem & Biomol Engn, Berkeley, CA 94720 USA.
[Lum, Yanwei; Ager, Joel W., III] Univ Calif Berkeley, Dept Mat Sci & Engn, Berkeley, CA 94720 USA.
RP Bell, AT (reprint author), Lawrence Berkeley Natl Lab, Div Mat Sci, Joint Ctr Artificial Photosynth, Berkeley, CA 94720 USA.; Bell, AT (reprint author), Univ Calif Berkeley, Dept Chem & Biomol Engn, Berkeley, CA 94720 USA.
EM alexbell@berkeley.edu
OI Singh, Meenesh/0000-0002-3638-8866
FU Office of Science of the U.S. Department of Energy [DE-SC0004993];
A*STAR
FX This material is based on the work performed by the Joint Center for
Artificial Photosynthesis, a DOE Energy Innovation Hub, supported
through the Office of Science of the U.S. Department of Energy under
Award number DE-SC0004993. Y.L. acknowledges the support of an A*STAR
National Science Scholarship.
NR 33
TC 4
Z9 4
U1 134
U2 134
PU AMER CHEMICAL SOC
PI WASHINGTON
PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA
SN 0002-7863
J9 J AM CHEM SOC
JI J. Am. Chem. Soc.
PD OCT 5
PY 2016
VL 138
IS 39
BP 13006
EP 13012
DI 10.1021/jacs.6b07612
PG 7
WC Chemistry, Multidisciplinary
SC Chemistry
GA DY2WF
UT WOS:000384952100045
PM 27626299
ER
PT J
AU Chen, CH
Abella, L
Ceron, MR
Guerrero-Ayala, MA
Rodriguez-Fortea, A
Olmstead, MM
Powers, XB
Balch, AL
Poblet, JM
Echegoyen, L
AF Chen, Chia-Hsiang
Abella, Laura
Ceron, Maira R.
Guerrero-Ayala, Miguel A.
Rodriguez-Fortea, Antonio
Olmstead, Marilyn M.
Powers, Xian B.
Balch, Alan L.
Poblet, Josep M.
Echegoyen, Luis
TI Zigzag Sc2C2 Carbide Cluster inside a [88]Fullerene Cage with One
Heptagon, Sc2C2@C-s(hept)-C-88: A Kinetically Trapped Fullerene Formed
by C-2 Insertion?
SO JOURNAL OF THE AMERICAN CHEMICAL SOCIETY
LA English
DT Article
ID ENDOHEDRAL METALLOFULLERENES; CRYSTALLOGRAPHIC CHARACTERIZATION;
FORMATION MECHANISM; ISOMERS; APPROXIMATION; CHLORINATION; COMPRESSION;
SHRINKAGE; CHEMISTRY; C96CL20
AB A non-isolated pentagon rule metallic carbide clusterfullerene containing a heptagonal ring, Sc2C2@C-s(hept)-C-88, was isolated from the raw soot obtained by electric arc vaporization of graphite rods packed with Sc2O3 and graphite powder under a helium atmosphere. The Sc2C2@C-s(hept)-C-88 was purified by multistage high-performance liquid chromatography (HPLC), cocrystallized with Ni(octaethylporphyrin), and characterized by single-crystal X-ray diffraction. The diffraction data revealed a zigzag Sc2C2 unit inside an unprecedented C-s(hept)-C-88 carbon cage containing 13 pentagons, 32 hexagons, and 1 heptagon. Calculations suggest that the observed nonclassical fullerene could be a kinetically trapped species derived from the recently reported Sc2C2@C-2v(9)-C-86 via a direct C-2 insertion.
C1 [Chen, Chia-Hsiang; Ceron, Maira R.; Guerrero-Ayala, Miguel A.; Echegoyen, Luis] Univ Texas El Paso, Dept Chem, El Paso, TX 79968 USA.
[Olmstead, Marilyn M.; Powers, Xian B.; Balch, Alan L.] Univ Calif Davis, Dept Chem, One Shields Ave, Davis, CA 95616 USA.
[Abella, Laura; Rodriguez-Fortea, Antonio; Poblet, Josep M.] Univ Rovira & Virgili, Dept Quim Fis & Inorgan, C Marcelli Domingo 1, E-43007 Tarragona, Spain.
[Chen, Chia-Hsiang] Leibniz Inst Solid State & Mat Res, Dept Electrochem & Conducting Polymers, D-01069 Dresden, Germany.
[Ceron, Maira R.] Lawrence Livermore Natl Lab, Phys & Life Sci, 7000 East Ave, Livermore, CA 94550 USA.
RP Echegoyen, L (reprint author), Univ Texas El Paso, Dept Chem, El Paso, TX 79968 USA.; Olmstead, MM; Balch, AL (reprint author), Univ Calif Davis, Dept Chem, One Shields Ave, Davis, CA 95616 USA.; Poblet, JM (reprint author), Univ Rovira & Virgili, Dept Quim Fis & Inorgan, C Marcelli Domingo 1, E-43007 Tarragona, Spain.
EM mmolmstead@ucdavis.edu; albalch@ucdavis.edu; josepmaria.poblet@urv.cat;
echegoyen@utep.edu
RI Chen, Chia-Hsiang/N-2224-2016; Poblet, Josep M./A-2739-2008;
Rodriguez-Fortea, Antonio/C-2688-2017
OI Poblet, Josep M./0000-0002-4533-0623; Rodriguez-Fortea,
Antonio/0000-0001-5884-5629
FU Robert A. Welch Foundation [AH-0033]; U.S. NSF [CHE-1408865,
CHE-1305125]; Office of Science, Office of Basic Energy Sciences, U.S.
Department of Energy [DE-AC02-05CH11231]; Spanish Ministerio de Ciencia
e Innovacion [CTQ2014-52774-P]; Generalitat de Catalunya [2014SGR-199,
XRQTC, FI-DGR 2014]; ICREA foundation; Department of Education
FX Dedicated to Prof. Tomas Torres on the occasion of his 65th birthday.
L.E. thanks the Robert A. Welch Foundation for an endowed chair and
Grant No. AH-0033 and the U.S. NSF (Grant No. CHE-1408865) for generous
financial support. A.L.B. and M.M.O. thank the U.S. NSF (Grant No.
CHE-1305125) generous financial support. We thank the Advanced Light
Source, supported by the Director, Office of Science, Office of Basic
Energy Sciences, U.S. Department of Energy under Contract No.
DE-AC02-05CH11231 for synchrotron beam time. This work was also
supported by the Spanish Ministerio de Ciencia e Innovacion (Project No.
CTQ2014-52774-P) and the Generalitat de Catalunya (2014SGR-199 and
XRQTC). J.M.P. thanks the ICREA foundation for an ICREA ACADEMIA award.
L.A. thanks the Generalitat de Catalunya for a predoctoral fellowship
(FI-DGR 2014). X.B.P. thanks the Department of Education for a GAANN
fellowship.
NR 58
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Z9 3
U1 26
U2 26
PU AMER CHEMICAL SOC
PI WASHINGTON
PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA
SN 0002-7863
J9 J AM CHEM SOC
JI J. Am. Chem. Soc.
PD OCT 5
PY 2016
VL 138
IS 39
BP 13030
EP 13037
DI 10.1021/jacs.6b07912
PG 8
WC Chemistry, Multidisciplinary
SC Chemistry
GA DY2WF
UT WOS:000384952100048
PM 27592501
ER
PT J
AU Ma, FS
Reichhardt, C
Gan, WL
Reichhardt, CJO
Lew, WS
AF Ma, Fusheng
Reichhardt, C.
Gan, Weiliang
Reichhardt, C. J. Olson
Lew, Wen Siang
TI Emergent geometric frustration of artificial magnetic skyrmion crystals
SO PHYSICAL REVIEW B
LA English
DT Article
ID CURRENT-DRIVEN DYNAMICS; SPIN-ICE; MNSI NANOWIRES; ROOM-TEMPERATURE;
WEAK FERROMAGNETISM; CLUSTER STATES; CHIRAL MAGNET; LATTICE; MOTION;
ENTROPY
AB Magnetic skyrmions have been receiving growing attention as potential information storage and magnetic logic devices since an increasing number of materials have been identified that support skyrmion phases. Explorations of artificial frustrated systems have led to new insights into controlling and engineering new emergent frustration phenomena in frustrated and disordered systems. Here, we propose a skyrmion spin ice, giving a unifying framework for the study of geometric frustration of skyrmion crystals (SCs) in a nonfrustrated artificial geometrical lattice as a consequence of the structural confinement of skyrmions in magnetic potential wells. The emergent ice rules from the geometrically frustrated SCs highlight a novel phenomenon in this skyrmion system: emergent geometrical frustration. We demonstrate how SC topology transitions between a nonfrustrated periodic configuration and a frustrated icelike ordering can also be realized reversibly. The proposed artificial frustrated skyrmion systems can be annealed into different ice phases with an applied current-induced spin-transfer torque, including a long-range ordered ice rule obeying ground state, as-relaxed random state, biased state, and monopole state. The spin-torque reconfigurability of the artificial skyrmion ice states, difficult to achieve in other artificial spin ice systems, is compatible with standard spintronic device fabrication technology, which makes the semiconductor industrial integration straightforward.
C1 [Ma, Fusheng; Gan, Weiliang; Lew, Wen Siang] Nanyang Technol Univ, Sch Phys & Math Sci, 21 Nanyang Link, Singapore 637371, Singapore.
[Reichhardt, C.; Reichhardt, C. J. Olson] Los Alamos Natl Lab, Div Theoret, Los Alamos, NM 87545 USA.
[Reichhardt, C.; Reichhardt, C. J. Olson] Los Alamos Natl Lab, Ctr Nonlinear Studies, Los Alamos, NM 87545 USA.
RP Lew, WS (reprint author), Nanyang Technol Univ, Sch Phys & Math Sci, 21 Nanyang Link, Singapore 637371, Singapore.
EM wensiang@ntu.edu.sg
RI Ma, Fusheng/I-5267-2013; Lew, Wen Siang/C-2910-2008;
OI Ma, Fusheng/0000-0002-2290-8744; Lew, Wen Siang/0000-0002-5161-741X;
Reichhardt, Cynthia/0000-0002-3487-5089
FU Singapore National Research Foundation, Prime Minister's Office
[NRF-CRP9-2011-01, NRF2015-IIP001-001]; MOE-AcRF Tier 2 Grant [MOE
2013-T2-2-017]
FX This paper was supported by the Singapore National Research Foundation,
Prime Minister's Office, under a Competitive Research Programme
(Non-volatile Magnetic Logic and Memory Integrated Circuit Devices, No.
NRF-CRP9-2011-01), and an Industry-IHL Partnership Program (No.
NRF2015-IIP001-001). The paper was also supported by a MOE-AcRF Tier 2
Grant (No. MOE 2013-T2-2-017). W.S.L. is a member of the Singapore
Spintronics Consortium (SG-SPIN).
NR 104
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Z9 0
U1 22
U2 22
PU AMER PHYSICAL SOC
PI COLLEGE PK
PA ONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA
SN 2469-9950
EI 2469-9969
J9 PHYS REV B
JI Phys. Rev. B
PD OCT 5
PY 2016
VL 94
IS 14
AR 144405
DI 10.1103/PhysRevB.94.144405
PG 11
WC Physics, Condensed Matter
SC Physics
GA DY6MB
UT WOS:000385240300002
ER
PT J
AU Mustafa, JI
Bernardi, M
Neaton, JB
Louie, SG
AF Mustafa, Jamal I.
Bernardi, Marco
Neaton, Jeffrey B.
Louie, Steven G.
TI Ab initio electronic relaxation times and transport in noble metals
SO PHYSICAL REVIEW B
LA English
DT Article
ID ELECTRICAL-RESISTIVITY; PHONON INTERACTIONS; FERMI SURFACES; TETRAHEDRON
METHOD; WANNIER FUNCTIONS; QUASI-PARTICLE; COPPER; SILVER; GOLD
AB Relaxation times employed to study electron transport inmetals are typically taken to be constants and obtained empirically. Here, we use fully ab initio calculations to compute the electron-phonon relaxation times of Cu, Ag, and Au and find that they vary significantly on the Fermi surface, with values from similar to 15 to 45 fs that are correlated with the Fermi surface topology. We compute room-temperature resistivities in excellent agreement with experiment by combining GW quasiparticle band structures, Wannier-interpolated band velocities, and ab initio relaxation times. We introduce an importance sampling scheme to speed up the convergence of resistivity and transport calculations.
C1 [Mustafa, Jamal I.; Bernardi, Marco; Neaton, Jeffrey B.; Louie, Steven G.] Univ Calif Berkeley, Dept Phys, Berkeley, CA 94720 USA.
[Mustafa, Jamal I.; Bernardi, Marco; Neaton, Jeffrey B.; Louie, Steven G.] Lawrence Berkeley Natl Lab, Div Mat Sci, Berkeley, CA 94720 USA.
[Bernardi, Marco] CALTECH, Dept Appl Phys & Mat Sci, Pasadena, CA 91125 USA.
[Neaton, Jeffrey B.] Lawrence Berkeley Natl Lab, Mol Foundry, Berkeley, CA 94720 USA.
[Neaton, Jeffrey B.] Kavli Energy NanoSci Inst Berkeley, Berkeley, CA 94720 USA.
RP Louie, SG (reprint author), Univ Calif Berkeley, Dept Phys, Berkeley, CA 94720 USA.; Louie, SG (reprint author), Lawrence Berkeley Natl Lab, Div Mat Sci, Berkeley, CA 94720 USA.
EM sglouie@berkeley.edu
FU Theory of Materials Program at the Lawrence Berkeley National Laboratory
through the Office of Basic Energy Sciences, U.S. Department of Energy
[DE-AC02-05CH11231]; National Science Foundation [DMR-1508412]; Office
of Science, Office of Basic Energy Sciences; U.S. Department of Energy
[DE-AC02-05CH11231]; Office of Science of the U.S. Department of Energy
[DE-AC02-05CH11231]
FX This research was supported by the Theory of Materials Program at the
Lawrence Berkeley National Laboratory through the Office of Basic Energy
Sciences, U.S. Department of Energy, under Contract No.
DE-AC02-05CH11231, which provided the GW calculations and scattering
rate simulations, and by the National Science Foundation under Grant No.
DMR-1508412, which provided for basic theory and electron-phonon
coupling matrix element calculations. Work at the Molecular Foundry was
supported by the Office of Science, Office of Basic Energy Sciences, and
by the U.S. Department of Energy under Contract No. DE-AC02-05CH11231.
This research used resources of the National Energy Research Scientific
Computing Center, a DOE Office of Science User Facility supported by the
Office of Science of the U.S. Department of Energy under Contract No.
DE-AC02-05CH11231.
NR 46
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U1 9
U2 9
PU AMER PHYSICAL SOC
PI COLLEGE PK
PA ONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA
SN 2469-9950
EI 2469-9969
J9 PHYS REV B
JI Phys. Rev. B
PD OCT 5
PY 2016
VL 94
IS 15
AR 155105
DI 10.1103/PhysRevB.94.155105
PG 5
WC Physics, Condensed Matter
SC Physics
GA DY6ML
UT WOS:000385241300001
ER
PT J
AU Quashie, EE
Saha, BC
Correa, AA
AF Quashie, Edwin E.
Saha, Bidhan C.
Correa, Alfredo A.
TI Electronic band structure effects in the stopping of protons in copper
SO PHYSICAL REVIEW B
LA English
DT Article
ID MOLECULAR-DYNAMICS; IONS; ENERGY; MATTER; ATOMS; POWER
AB We present an ab initio study of the electronic stopping power of protons in copper over a wide range of proton velocities v = 0.02-10 a.u. where we take into account nonlinear effects. Time-dependent density functional theory coupled with molecular dynamics is used to study electronic excitations produced by energetic protons. A plane-wave pseudopotential scheme is employed to solve the time-dependent Kohn-Sham equations for a moving ion in a periodic crystal. The electronic excitations and the band structure determine the stopping power of the material and alter the interatomic forces for both channeling and off-channeling trajectories. Our off-channeling results are in quantitative agreement with experiments, and at low velocity they unveil a crossover region of superlinear velocity dependence (with a power of similar to 1.5) in the velocity range v = 0.07-0.3 a.u., which we associate to the copper crystalline electronic band structure. The results are rationalized by simple band models connecting two separate regimes. We find that the limit of electronic stopping v. 0 is not as simple as phenomenological models suggest and it is plagued by band-structure effects.
C1 [Quashie, Edwin E.; Saha, Bidhan C.] Florida A&M Univ, Dept Phys, Tallahassee, FL 32307 USA.
[Correa, Alfredo A.] Lawrence Livermore Natl Lab, 7000 East Ave, Livermore, CA 94550 USA.
RP Quashie, EE (reprint author), Florida A&M Univ, Dept Phys, Tallahassee, FL 32307 USA.
FU U.S. Department of Energy by Lawrence Livermore National Laboratory
[DE-AC52-07NA27344]; National Nuclear Security Administration (NNSA)
[DE-NA0002630]
FX We would like to thank Professor C. A. Weatherford, Dr. E. R. Schwegler,
and Dr. K. J. Reed for their keen interest, constant encouragement, and
useful suggestions throughout the progress of this paper. This work was
performed under the auspices of the U.S. Department of Energy by
Lawrence Livermore National Laboratory under Contract DE-AC52-07NA27344.
Computing support for this work came from the Lawrence Livermore
National Laboratory Institutional Computing Grand Challenge program.
This is a collaborative project between the Department of Physics,
Florida A&M University, and Lawrence Livermore National Laboratory.
E.E.Q. and B.C.S. thankfully acknowledge the support by National Nuclear
Security Administration (NNSA), Award No. DE-NA0002630.
NR 61
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U1 3
U2 3
PU AMER PHYSICAL SOC
PI COLLEGE PK
PA ONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA
SN 2469-9950
EI 2469-9969
J9 PHYS REV B
JI Phys. Rev. B
PD OCT 5
PY 2016
VL 94
IS 15
AR 155403
DI 10.1103/PhysRevB.94.155403
PG 7
WC Physics, Condensed Matter
SC Physics
GA DY6ML
UT WOS:000385241300005
ER
PT J
AU Schweitzer, P
Weiss, C
AF Schweitzer, P.
Weiss, C.
TI Spin-flavor structure of chiral-odd generalized parton distributions in
the large-N-c limit
SO PHYSICAL REVIEW C
LA English
DT Article
ID HARD EXCLUSIVE ELECTROPRODUCTION; VIRTUAL COMPTON-SCATTERING; 2
VECTOR-MESONS; MASS SPLITTINGS; NUCLEON; QCD; TRANSVERSITY; SOLITON;
BARYONS; PHOTOPRODUCTION
AB We study the spin-flavor structure of the nucleon's chiral-odd generalized parton distributions (transversity GPDs) in the large-N-c limit of QCD. In contrast to the chiral-even case, only three combinations of the four chiral-odd GPDs are nonzero in the leading order of the 1/N-c expansion: (E) over bar (T) = E-T + 2 (H) over tilde (T), H-T, and (E) over tilde (T). The degeneracy is explained by the absence of spin-orbit interactions correlating the transverse momentum transfer with the transverse quark spin. It can also be deduced from the natural N-c scaling of the quark-nucleon helicity amplitudes associated with the GPDs. In the GPD (E) over bar (T) the flavor-singlet component u + d is leading in the 1/N-c expansion, while in HT and (E) over tilde (T) it is the flavor-nonsinglet components u - d. The large-Nc relations are consistent with the spin-flavor structure extracted from hard exclusive pi(0) and eta electroproduction data, if it is assumed that the processes are mediated by twist-3 amplitudes involving the chiral-odd GPDs and the chiral-odd pseudoscalar meson distribution amplitudes.
C1 [Schweitzer, P.] Univ Tubingen, Inst Theoret Phys, Morgenstelle 14, D-72076 Tubingen, Germany.
[Schweitzer, P.] Univ Connecticut, Dept Phys, Storrs, CT 06269 USA.
[Weiss, C.] Jefferson Lab, Ctr Theory, Newport News, VA 23606 USA.
RP Schweitzer, P (reprint author), Univ Tubingen, Inst Theoret Phys, Morgenstelle 14, D-72076 Tubingen, Germany.; Schweitzer, P (reprint author), Univ Connecticut, Dept Phys, Storrs, CT 06269 USA.
EM peter.schweitzer@phys.uconn.edu; weiss@jlab.org
FU U.S. Department of Energy, Office of Science, Office of Nuclear Physics
[DE-AC05-06OR23177]; U.S. National Science Foundation [1406298];
Deutsche Forschungsgemeinschaft [VO 1049/1]
FX In this study we greatly benefited from discussions with D. Diakonov, V.
Petrov, P. Pobylitsa, and M. Polyakov during earlier joint work. This
material is based upon work supported by the U.S. Department of Energy,
Office of Science, Office of Nuclear Physics under Contract No.
DE-AC05-06OR23177. This work was supported by the U.S. National Science
Foundation under Contract No. 1406298, and by the Deutsche
Forschungsgemeinschaft (Grant No. VO 1049/1).
NR 61
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U1 0
U2 0
PU AMER PHYSICAL SOC
PI COLLEGE PK
PA ONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA
SN 2469-9985
EI 2469-9993
J9 PHYS REV C
JI Phys. Rev. C
PD OCT 5
PY 2016
VL 94
IS 4
AR 045202
DI 10.1103/PhysRevC.94.045202
PG 10
WC Physics, Nuclear
SC Physics
GA DY6NQ
UT WOS:000385244400001
ER
PT J
AU Harigaya, K
Nomura, Y
AF Harigaya, Keisuke
Nomura, Yasunori
TI Hidden pion varieties in composite models for diphoton resonances
SO PHYSICAL REVIEW D
LA English
DT Article
ID GAUGE-THEORIES; BOSON
AB The diphoton excesses at 750 GeV seen in the LHC data may be the first hint of new physics at the TeV scale. We discuss variations of the model considered earlier, in which one or more diphoton excesses arise from composite pseudo-Nambu-Goldstone bosons (hidden pions) associated with new strong dynamics at the TeV scale. We study the case in which the 750 GeV excess arises from a unique hidden pion leading to a diphoton final state as well as the case in which it arises from one of the hidden pions decaying into diphotons. We consider SU(N), SO(N), and Sp(N) gauge groups for the strong dynamics and find that SO(N) and Sp(N) models give extra hidden pions beyond those in the SU(N) models, which can be used to discriminate among models.
C1 [Harigaya, Keisuke] Univ Calif Berkeley, Berkeley Ctr Theoret Phys, Dept Phys, Berkeley, CA 94720 USA.
Lawrence Berkeley Natl Lab, Theoret Phys Grp, Berkeley, CA 94720 USA.
RP Harigaya, K (reprint author), Univ Calif Berkeley, Berkeley Ctr Theoret Phys, Dept Phys, Berkeley, CA 94720 USA.
FU Department of Energy, Office of Science, Office of High Energy Physics
[DE-AC02-05CH11231]; National Science Foundation [PHY-1316783,
PHY-1521446]; MEXT KAKENHI [15H05895]
FX This work was supported in part by the Department of Energy, Office of
Science, Office of High Energy Physics, under Contract No.
DE-AC02-05CH11231, by the National Science Foundation under Grants No.
PHY-1316783 and No. PHY-1521446, and by MEXT KAKENHI Grant No. 15H05895.
NR 42
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U1 0
U2 0
PU AMER PHYSICAL SOC
PI COLLEGE PK
PA ONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA
SN 2470-0010
EI 2470-0029
J9 PHYS REV D
JI Phys. Rev. D
PD OCT 5
PY 2016
VL 94
IS 7
AR 075004
DI 10.1103/PhysRevD.94.075004
PG 12
WC Astronomy & Astrophysics; Physics, Particles & Fields
SC Astronomy & Astrophysics; Physics
GA DY6OA
UT WOS:000385245400003
ER
PT J
AU Campione, S
Marquier, F
Hugonin, JP
Ellis, AR
Klem, JF
Sinclair, MB
Luk, TS
AF Campione, Salvatore
Marquier, Francois
Hugonin, Jean-Paul
Ellis, A. Robert
Klem, John F.
Sinclair, Michael B.
Luk, Ting S.
TI Directional and monochromatic thermal emitter from epsilon-near-zero
conditions in semiconductor hyperbolic metamaterials
SO SCIENTIFIC REPORTS
LA English
DT Article
ID OPTICAL-PROPERTIES; EMISSION; BAND
AB The development of novel thermal sources that control the emission spectrum and the angular emission pattern is of fundamental importance. In this paper, we investigate the thermal emission properties of semiconductor hyperbolic metamaterials (SHMs). Our structure does not require the use of any periodic corrugation to provide monochromatic and directional emission properties. We show that these properties arise because of epsilon-near-zero conditions in SHMs. The thermal emission is dominated by the epsilon-near-zero effect in the doped quantum wells composing the SHM. Furthermore, different properties are observed for s and p polarizations, following the characteristics of the strong anisotropy of hyperbolic metamaterials.
C1 [Campione, Salvatore; Ellis, A. Robert; Klem, John F.; Sinclair, Michael B.; Luk, Ting S.] Sandia Natl Labs, POB 5800, Albuquerque, NM 87185 USA.
[Campione, Salvatore; Luk, Ting S.] Sandia Natl Labs, Ctr Integrated Nanotechnol CINT, POB 5800, Albuquerque, NM 87185 USA.
[Marquier, Francois; Hugonin, Jean-Paul] Univ Paris 11, CNRS, Inst Opt, Lab Charles Fabry, Campus Polytech,RD128, F-91127 Palaiseau, France.
RP Campione, S; Luk, TS (reprint author), Sandia Natl Labs, POB 5800, Albuquerque, NM 87185 USA.; Campione, S; Luk, TS (reprint author), Sandia Natl Labs, Ctr Integrated Nanotechnol CINT, POB 5800, Albuquerque, NM 87185 USA.
EM sncampi@sandia.gov; tsluk@sandia.gov
FU US. Department of Energy, Office of Basic Energy Sciences, Division of
Materials Sciences and Engineering; US. Department of Energy's National
Nuclear Security Administration [DE-AC04-94AL85000]; French Ministry of
Defense through Direction Generale de l'Armement (DGA) [ERE
2014.60.0082]
FX This work was supported by the US. Department of Energy, Office of Basic
Energy Sciences, Division of Materials Sciences and Engineering and
performed, in part, at the Center for Integrated Nanotechnologies, an
Office of Science User Facility operated for the US. Department of
Energy (DOE) Office of Science. Sandia National Laboratories is a
multi-mission laboratory managed and operated by Sandia Corporation, a
wholly owned subsidiary of Lockheed Martin Corporation, for the US.
Department of Energy's National Nuclear Security Administration under
contract DE-AC04-94AL85000. F. M. acknowledges financial support from
the French Ministry of Defense through the grant ERE 2014.60.0082 from
the Direction Generale de l'Armement (DGA).
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PI LONDON
PA MACMILLAN BUILDING, 4 CRINAN ST, LONDON N1 9XW, ENGLAND
SN 2045-2322
J9 SCI REP-UK
JI Sci Rep
PD OCT 5
PY 2016
VL 6
AR 34746
DI 10.1038/srep34746
PG 9
WC Multidisciplinary Sciences
SC Science & Technology - Other Topics
GA DX8RX
UT WOS:000384657900001
PM 27703223
ER
PT J
AU Mehdi, BL
Stevens, A
Qian, JF
Park, C
Xu, W
Henderson, WA
Zhang, JG
Mueller, KT
Browning, ND
AF Mehdi, B. Layla
Stevens, Andrew
Qian, Jiangfeng
Park, Chiwoo
Xu, Wu
Henderson, Wesley A.
Zhang, Ji-Guang
Mueller, Karl T.
Browning, Nigel D.
TI The Impact of Li Grain Size on Coulombic Efficiency in Li Batteries
SO SCIENTIFIC REPORTS
LA English
DT Article
ID TRANSMISSION ELECTRON-MICROSCOPY; LITHIUM-ION BATTERIES; LIQUID-CELL;
GROWTH; METAL; DEPOSITION; ANODES; NANOPARTICLES; MECHANISMS; CHALLENGES
AB One of the most promising means to increase the energy density of state-of-the-art lithium Li-ion batteries is to replace the graphite anode with a Li metal anode. While the direct use of Li metal may be highly advantageous, at present its practical application is limited by issues related to dendrite growth and low Coulombic efficiency, CE. Here operando electrochemical scanning transmission electron microscopy (STEM) is used to directly image the deposition/stripping of Li at the anode-electrolyte interface in a Li-based battery. A non-aqueous electrolyte containing small amounts of H2O as an additive results in remarkably different deposition/stripping properties as compared to the "dry" electrolyte when operated under identical electrochemical conditions. The electrolyte with the additive deposits more Li during the first cycle, with the grain sizes of the Li deposits being significantly larger and more variable. The stripping of the Li upon discharge is also more complete, i.e., there is a higher cycling CE. This suggests that larger grain sizes are indicative of better performance by leading to more uniform Li deposition and an overall decrease in the formation of Li dendrites and side reactions with electrolyte components, thus potentially paving the way for the direct use of Li metal in battery technologies.
C1 [Mehdi, B. Layla; Qian, Jiangfeng; Xu, Wu; Zhang, Ji-Guang; Mueller, Karl T.; Browning, Nigel D.] PNNL, JCESR, Richland, WA 99352 USA.
[Mehdi, B. Layla; Browning, Nigel D.] PNNL, Phys & Computat Sci Directorate, Richland, WA 99352 USA.
[Stevens, Andrew] PNNL, Natl Secur Directorate, Richland, WA 99352 USA.
[Qian, Jiangfeng; Xu, Wu; Henderson, Wesley A.; Zhang, Ji-Guang] PNNL, Energy & Environm Directorate, Richland, WA 99352 USA.
[Park, Chiwoo] Florida State Univ, Ind & Mfg Engn, Tallahassee, FL 32306 USA.
[Mueller, Karl T.] PNNL, Environm Mol Sci Lab, Richland, WA 99352 USA.
[Mueller, Karl T.] Penn State Univ, Dept Chem, University Pk, PA 16802 USA.
[Browning, Nigel D.] Univ Washington, Mat Sci & Engn, Seattle, WA 98195 USA.
RP Mehdi, BL; Browning, ND (reprint author), PNNL, JCESR, Richland, WA 99352 USA.; Mehdi, BL; Browning, ND (reprint author), PNNL, Phys & Computat Sci Directorate, Richland, WA 99352 USA.; Browning, ND (reprint author), Univ Washington, Mat Sci & Engn, Seattle, WA 98195 USA.
EM Layla.Mehdi@pnnl.gov; Nigel.Browning@pnnl.gov
OI Stevens, Andrew/0000-0002-8474-8483; Xu, Wu/0000-0002-2685-8684
FU Joint Center for Energy Storage Research (JCESR), an Energy Innovation
Hub - Department of Energy, Office of Science, Basic Energy Sciences;
Chemical Imaging Initiative, a Laboratory Directed Research and
Development Program at Pacific Northwest National Laboratory (PNNL);
U.S. Department of Energy (DOE) [DE-AC05-76RL01830]; Department of
Energy's Office of Biological and Environmental Research at PNNL;
National Science Foundation [NSF-1334012]
FX This work was primarily supported by Joint Center for Energy Storage
Research (JCESR), an Energy Innovation Hub funded by the Department of
Energy, Office of Science, Basic Energy Sciences. The development of the
operando stage was supported by the Chemical Imaging Initiative, a
Laboratory Directed Research and Development Program at Pacific
Northwest National Laboratory (PNNL). PNNL is a multi-program national
laboratory operated by Battelle for the U.S. Department of Energy (DOE)
under Contract DE-AC05-76RL01830. A portion of the research was
performed using the Environmental Molecular Sciences Laboratory (EMSL),
a national scientific user facility sponsored by the Department of
Energy's Office of Biological and Environmental Research and located at
PNNL. The development of the multi-target tracking algorithm is
supported by the National Science Foundation under NSF-1334012.
NR 30
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PU NATURE PUBLISHING GROUP
PI LONDON
PA MACMILLAN BUILDING, 4 CRINAN ST, LONDON N1 9XW, ENGLAND
SN 2045-2322
J9 SCI REP-UK
JI Sci Rep
PD OCT 5
PY 2016
VL 6
AR 34267
DI 10.1038/srep34267
PG 8
WC Multidisciplinary Sciences
SC Science & Technology - Other Topics
GA DX8RW
UT WOS:000384657800002
PM 27703188
ER
PT J
AU Theiler, J
Yoon, H
Yusim, K
Picker, LJ
Fruh, K
Korber, B
AF Theiler, James
Yoon, Hyejin
Yusim, Karina
Picker, Louis J.
Fruh, Klaus
Korber, Bette
TI Epigraph: A Vaccine Design Tool Applied to an HIV Therapeutic Vaccine
and a Pan-Filovirus Vaccine
SO SCIENTIFIC REPORTS
LA English
DT Article
ID T-LYMPHOCYTE RESPONSES; RHESUS-MONKEYS; IMMUNE-RESPONSES; MOSAIC
VACCINES; CELL RESPONSES; VIRUS; INFECTION; VARIANTS; COVERAGE; STRAINS
AB Epigraph is an efficient graph-based algorithm for designing vaccine antigens to optimize potential T-cell epitope (PTE) coverage. Epigraph vaccine antigens are functionally similar to Mosaic vaccines, which have demonstrated effectiveness in preliminary HIV non-human primate studies. In contrast to the Mosaic algorithm, Epigraph is substantially faster, and in restricted cases, provides a mathematically optimal solution. Epigraph furthermore has new features that enable enhanced vaccine design flexibility. These features include the ability to exclude rare epitopes from a design, to optimize population coverage based on inexact epitope matches, and to apply the code to both aligned and unaligned input sequences. Epigraph was developed to provide practical design solutions for two outstanding vaccine problems. The first of these is a personalized approach to a therapeutic T-cell HIV vaccine that would provide antigens with an excellent match to an individual's infecting strain, intended to contain or clear a chronic infection. The second is a pan-filovirus vaccine, with the potential to protect against all known viruses in the Filoviradae family, including ebolaviruses. A web-based interface to run the Epigraph tool suite is available (http://www.hiv.lanl.gov/content/sequence/EPIGRAPH/epigraph.html).
C1 [Theiler, James; Yoon, Hyejin; Yusim, Karina; Korber, Bette] Los Alamos Natl Lab, Los Alamos, NM 87545 USA.
[Theiler, James; Yusim, Karina; Korber, Bette] New Mexico Consortium, Los Alamos, NM 87544 USA.
[Picker, Louis J.; Fruh, Klaus] Oregon Hlth & Sci Univ, Portland, OR 97239 USA.
RP Korber, B (reprint author), Los Alamos Natl Lab, Los Alamos, NM 87545 USA.; Korber, B (reprint author), New Mexico Consortium, Los Alamos, NM 87544 USA.
EM btk@lanl.gov
FU National Institute of Allergy and Infectious Diseases award NIAID [2 R44
AI100343-02]; National Institute of Allergy and Infectious Diseases
award CHAVI-ID; Center for HIV/AIDS Vaccine Immunology and Immunogen
Discovery [UM1-AI100645]; Bill and Melinda Gates Foundation Global
Health Proposal [OPP1108533]; Royalty Funds from Los Alamos National
Laboratory
FX This work was funded through: National Institute of Allergy and
Infectious Diseases awards NIAID 2 R44 AI100343-02, and CHAVI-ID;
UM1-AI100645, the Center for HIV/AIDS Vaccine Immunology and Immunogen
Discovery; The Bill and Melinda Gates Foundation Global Health Proposal
OPP1108533; and Royalty Funds from Los Alamos National Laboratory. We
thank Goutam Gupta, Jose Olivares, and Jurgen Schmidt (LANL) for their
efforts to make the Ebola work possible through internal Los Alamos
funding. We thank Tomas Hanke and Andrew McMichael (Oxford), and Barton
Haynes and Larry Liao (Duke), for thoughtful advice regarding the design
of the pan-Filovirus T-cell vaccine. We thank Aric Hagberg, Misha
Chertkov, and Diane Oyen for useful discussions about graph-theoretic
algorithms, and the authors of the NetworkX library for making the
source code freely available.
NR 50
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PI LONDON
PA MACMILLAN BUILDING, 4 CRINAN ST, LONDON N1 9XW, ENGLAND
SN 2045-2322
J9 SCI REP-UK
JI Sci Rep
PD OCT 5
PY 2016
VL 6
AR 33987
DI 10.1038/srep33987
PG 15
WC Multidisciplinary Sciences
SC Science & Technology - Other Topics
GA DX8RB
UT WOS:000384655500001
PM 27703185
ER
PT J
AU Yang, CY
Li, Y
Zhou, YY
Lei, XQ
Zheng, W
Tian, Y
Van Nostrand, JD
He, ZL
Wu, LY
Zhou, JZ
Zheng, TL
AF Yang, Caiyun
Li, Yi
Zhou, Yanyan
Lei, Xueqian
Zheng, Wei
Tian, Yun
Van Nostrand, Joy D.
He, Zhili
Wu, Liyou
Zhou, Jizhong
Zheng, Tianling
TI A comprehensive insight into functional profiles of free-living
microbial community responses to a toxic Akashiwo sanguinea bloom
SO SCIENTIFIC REPORTS
LA English
DT Article
ID SPRING PHYTOPLANKTON BLOOM; GEOCHIP-BASED ANALYSIS; HARMFUL ALGAL BLOOM;
SEA OIL PLUME; BACTERIAL COMMUNITY; MARINE-PHYTOPLANKTON;
ALEXANDRIUM-TAMARENSE; GENE DIVERSITY; DIATOM BLOOM; CELL-DEATH
AB Phytoplankton blooms are a worldwide problem and can greatly affect ecological processes in aquatic systems, but its impacts on the functional potential of microbial communities are limited. In this study, a high-throughput microarray-based technology (GeoChip) was used to profile the functional potential of free-living microbes from the Xiamen Sea Area in response to a 2011 Akashiwo sanguinea bloom. The bloom altered the overall community functional structure. Genes that were significantly (p < 0.05) increased during the bloom included carbon degradation genes and genes involved in nitrogen (N) and/or phosphorus (P) limitation stress. Such significantly changed genes were well explained by chosen environmental factors (COD, nitrite-N, nitrate-N, dissolved inorganic phosphorus, chlorophyll-a and algal density). Overall results suggested that this bloom might enhance the microbial converting of nitrate to N-2 and ammonia nitrogen, decrease P removal from seawater, activate the glyoxylate cycle, and reduce infection activity of bacteriophage. This study presents new information on the relationship of algae to other microbes in aquatic systems, and provides new insights into our understanding of ecological impacts of phytoplankton blooms.
C1 [Yang, Caiyun] Southwest Univ, Coll Resources & Environm, Res Ctr Bioenergy & Bioremediat, Chongqing, Peoples R China.
[Yang, Caiyun; Zhou, Yanyan; Lei, Xueqian; Zheng, Wei; Tian, Yun; Zheng, Tianling] Xiamen Univ, Sch Life Sci, State Key Lab Marine Environm Sci, Xiamen 361005, Peoples R China.
[Yang, Caiyun; Li, Yi; Zhou, Yanyan; Lei, Xueqian; Zheng, Wei; Tian, Yun; Zheng, Tianling] Xiamen Univ, Sch Life Sci, Key Lab, Minist Educ Coastal & Wetland Ecosyst, Xiamen 361005, Peoples R China.
[Li, Yi] Henan Normal Univ, Coll Life Sci, Xinxiang, Peoples R China.
[Van Nostrand, Joy D.; He, Zhili; Wu, Liyou; Zhou, Jizhong] Univ Oklahoma, Inst Environm Genom, Norman, OK 73019 USA.
[Van Nostrand, Joy D.; He, Zhili; Wu, Liyou; Zhou, Jizhong] Univ Oklahoma, Dept Microbiol & Plant Biol, Norman, OK 73019 USA.
[Zhou, Jizhong] Lawrence Berkeley Natl Lab, Div Earth Sci, Berkeley, CA 94720 USA.
[Zhou, Jizhong] Tsinghua Univ, Sch Environm, Beijing 100084, Peoples R China.
RP Zheng, TL (reprint author), Xiamen Univ, Sch Life Sci, State Key Lab Marine Environm Sci, Xiamen 361005, Peoples R China.; Zheng, TL (reprint author), Xiamen Univ, Sch Life Sci, Key Lab, Minist Educ Coastal & Wetland Ecosyst, Xiamen 361005, Peoples R China.; Zhou, JZ (reprint author), Univ Oklahoma, Inst Environm Genom, Norman, OK 73019 USA.; Zhou, JZ (reprint author), Univ Oklahoma, Dept Microbiol & Plant Biol, Norman, OK 73019 USA.; Zhou, JZ (reprint author), Lawrence Berkeley Natl Lab, Div Earth Sci, Berkeley, CA 94720 USA.; Zhou, JZ (reprint author), Tsinghua Univ, Sch Environm, Beijing 100084, Peoples R China.
EM jzhou@ou.edu; wshwzh@xmu.edu.cn
FU National Nature Science Foundation of China [41576109, 41376119,
31500095, 40930847]
FX This work was financed by the National Nature Science Foundation of
China (Nos: 41576109, 41376119, 31500095, 40930847), are gratefully
acknowledged.
NR 56
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PI LONDON
PA MACMILLAN BUILDING, 4 CRINAN ST, LONDON N1 9XW, ENGLAND
SN 2045-2322
J9 SCI REP-UK
JI Sci Rep
PD OCT 5
PY 2016
VL 6
AR 34645
DI 10.1038/srep34645
PG 10
WC Multidisciplinary Sciences
SC Science & Technology - Other Topics
GA DX8QJ
UT WOS:000384653500001
PM 27703234
ER
PT J
AU Shah, NH
Wang, Q
Yan, QR
Karandur, D
Kadlecek, TA
Fallahee, IR
Russ, WP
Ranganathan, R
Weiss, A
Kuriyan, J
AF Shah, Neel H.
Wang, Qi
Yan, Qingrong
Karandur, Deepti
Kadlecek, Theresa A.
Fallahee, Ian R.
Russ, William P.
Ranganathan, Rama
Weiss, Arthur
Kuriyan, John
TI An electrostatic selection mechanism controls sequential kinase
signaling downstream of the T cell receptor
SO ELIFE
LA English
DT Article
ID PROTEIN-TYROSINE KINASE; BROWNIAN DYNAMICS; STRUCTURAL BASIS;
INTERMOLECULAR AUTOPHOSPHORYLATION; TRANS-PHOSPHORYLATION; CATALYTIC
SPECIFICITY; INTERACTION NETWORK; INSULIN-RECEPTOR; FAMILY KINASES;
ZETA-CHAIN
AB The sequence of events that initiates T cell signaling is dictated by the specificities and order of activation of the tyrosine kinases that signal downstream of the T cell receptor. Using a platform that combines exhaustive point-mutagenesis of peptide substrates, bacterial surface display, cell sorting, and deep sequencing, we have defined the specificities of the first two kinases in this pathway, Lck and ZAP-70, for the T cell receptor chain and the scaffold proteins LAT and SLP-76. We find that ZAP-70 selects its substrates by utilizing an electrostatic mechanism that excludes substrates with positively-charged residues and favors LAT and SLP-76 phosphosites that are surrounded by negatively-charged residues. This mechanism prevents ZAP-70 from phosphorylating its own activation loop, thereby enforcing its strict dependence on Lck for activation. The sequence features in ZAP-70, LAT, and SLP-76 that underlie electrostatic selectivity likely contribute to the specific response of T cells to foreign antigens.
C1 [Shah, Neel H.; Wang, Qi; Yan, Qingrong; Karandur, Deepti; Fallahee, Ian R.; Kuriyan, John] Univ Calif Berkeley, Dept Mol & Cell Biol, 229 Stanley Hall, Berkeley, CA 94720 USA.
[Shah, Neel H.; Wang, Qi; Yan, Qingrong; Karandur, Deepti; Fallahee, Ian R.; Kuriyan, John] Univ Calif Berkeley, Calif Inst Quantitat Biosci, Berkeley, CA 94720 USA.
[Shah, Neel H.; Wang, Qi; Yan, Qingrong; Karandur, Deepti; Fallahee, Ian R.; Kuriyan, John] Univ Calif Berkeley, Howard Hughes Med Inst, Berkeley, CA 94720 USA.
[Kadlecek, Theresa A.; Weiss, Arthur] Univ Calif San Francisco, Dept Med, Rosalind Russell Ephraim P Engleman Rheumatol Res, San Francisco, CA USA.
[Kadlecek, Theresa A.; Weiss, Arthur] Univ Calif San Francisco, Howard Hughes Med Inst, San Francisco, CA USA.
[Russ, William P.; Ranganathan, Rama] Univ Texas Southwestern Med Ctr, Green Ctr Syst Biol, Dallas, TX USA.
[Ranganathan, Rama] Univ Texas Southwestern Med Ctr, Dept Biophys, Dallas, TX USA.
[Ranganathan, Rama] Univ Texas Southwestern Med Ctr, Dept Pharmacol, Dallas, TX USA.
[Kuriyan, John] Lawrence Berkeley Natl Lab, Mol Biophys & Integrated Bioimaging Div, Berkeley, CA USA.
[Wang, Qi] DE Shaw Res, New York, NY USA.
[Yan, Qingrong] Johnson & Johnson, Janssen Pharmaceut Co, Malvern, PA USA.
RP Kuriyan, J (reprint author), Univ Calif Berkeley, Dept Mol & Cell Biol, 229 Stanley Hall, Berkeley, CA 94720 USA.; Kuriyan, J (reprint author), Univ Calif Berkeley, Calif Inst Quantitat Biosci, Berkeley, CA 94720 USA.; Kuriyan, J (reprint author), Univ Calif Berkeley, Howard Hughes Med Inst, Berkeley, CA 94720 USA.; Kuriyan, J (reprint author), Lawrence Berkeley Natl Lab, Mol Biophys & Integrated Bioimaging Div, Berkeley, CA USA.
EM kuriyan@berkeley.edu
OI Weiss, Arthur/0000-0002-2414-9024
FU National Institutes of Health [PO1 AI091580]; Damon Runyon Cancer
Research Foundation; Cancer Research Institute
FX National Institutes of Health PO1 AI091580 Arthur Weiss John Kuriyan;
Damon Runyon Cancer Research Foundation Neel H Shah; Cancer Research
Institute Qi Wang Qingrong Yan
NR 96
TC 0
Z9 0
U1 6
U2 6
PU ELIFE SCIENCES PUBLICATIONS LTD
PI CAMBRIDGE
PA SHERATON HOUSE, CASTLE PARK, CAMBRIDGE, CB3 0AX, ENGLAND
SN 2050-084X
J9 ELIFE
JI eLife
PD OCT 4
PY 2016
VL 5
AR e20105
DI 10.7554/eLife.20105
PG 40
WC Biology
SC Life Sciences & Biomedicine - Other Topics
GA EB8UA
UT WOS:000387665400001
ER
PT J
AU Godsey, MH
Davulcu, O
Nix, JC
Skalicky, JJ
Bruschweiler, RP
Chapman, MS
AF Godsey, Michael H.
Davulcu, Omar
Nix, Jay C.
Skalicky, Jack J.
Bruschweiler, Rafael P.
Chapman, Michael S.
TI The Sampling of Conformational Dynamics in Ambient-Temperature Crystal
Structures of Arginine Kinase
SO STRUCTURE
LA English
DT Article
ID X-RAY CRYSTALLOGRAPHY; STATE ANALOG COMPLEX; INDUCED-FIT;
PROTEIN-STRUCTURE; RESOLUTION; MOTIONS; REFINEMENT; DOMAIN;
IDENTIFICATION; MOLECULES
AB Arginine kinase provides a model for functional dynamics, studied through crystallography, enzymology, and nuclear magnetic resonance. Structures are now solved, at ambient temperature, for the transition state analog (TSA) complex. Analysis of quasi-rigid sub-domain displacements show that differences between the two TSA structures average about 5% of changes between substrate-free and TSA forms, and they are nearly co-linear. Small backbone hinge rotations map to sites that also flex on substrate binding. Anisotropic atomic displacement parameters (ADPs) are refined using rigid-body TLS constraints. Consistency between crystal forms shows that they reflect intrinsic molecular properties more than crystal lattice effects. In many regions, the favored directions of thermal/static displacement are appreciably correlated with movements on substrate binding. Correlation between ADPs and larger substrate-associated movements implies that the latter approximately follow paths of low-energy intrinsic motions.
C1 [Godsey, Michael H.] Concordia Univ, Dept Math Sci, Portland, OR 97211 USA.
[Davulcu, Omar; Chapman, Michael S.] Oregon Hlth & Sci Univ, Sch Med, Dept Biochem & Mol Biol, Portland, OR 97239 USA.
[Nix, Jay C.] Lawrence Berkeley Natl Lab, Mol Biol Consortium, Berkeley, CA 94720 USA.
[Skalicky, Jack J.] Univ Utah, Sch Med, Dept Biochem, Salt Lake City, UT USA.
[Bruschweiler, Rafael P.] Ohio State Univ, Dept Chem & Biochem, Columbus, OH 43210 USA.
RP Chapman, MS (reprint author), Oregon Hlth & Sci Univ, Sch Med, Dept Biochem & Mol Biol, Portland, OR 97239 USA.
EM chapmami@ohsu.edu
FU NIH NIGMS [R01GM077643]
FX This work was supported by NIH NIGMS R01GM077643 (M.S.C.). Chiara del
Piccolo is thanked for calculations on RNase A.
NR 43
TC 0
Z9 0
U1 3
U2 3
PU CELL PRESS
PI CAMBRIDGE
PA 600 TECHNOLOGY SQUARE, 5TH FLOOR, CAMBRIDGE, MA 02139 USA
SN 0969-2126
EI 1878-4186
J9 STRUCTURE
JI Structure
PD OCT 4
PY 2016
VL 24
IS 10
BP 1658
EP 1667
DI 10.1016/j.str.2016.07.013
PG 10
WC Biochemistry & Molecular Biology; Biophysics; Cell Biology
SC Biochemistry & Molecular Biology; Biophysics; Cell Biology
GA EA6UF
UT WOS:000386763800006
PM 27594681
ER
PT J
AU Cross, JN
Macor, JA
Bertke, JA
Ferrier, MG
Girolami, GS
Kozimor, SA
Maassen, JR
Scott, BL
Shuh, DK
Stein, BW
Stieber, SCE
AF Cross, Justin N.
Macor, Joseph A.
Bertke, Jeffery A.
Ferrier, Maryline G.
Girolami, Gregory S.
Kozimor, Stosh A.
Maassen, Joel R.
Scott, Brian L.
Shuh, David K.
Stein, Benjamin W.
Stieber, S. Chantal E.
TI Comparing the 2,2 '-Biphenylenedithiophosphinate Binding of Americium
with Neodymium and Europium
SO ANGEWANDTE CHEMIE-INTERNATIONAL EDITION
LA English
DT Article
DE actinides; americium; lanthanides; radiochemistry; X-ray diffraction
ID SPECTROSCOPIC PROPERTIES; COORDINATION CHEMISTRY; HYDROTHERMAL
SYNTHESIS; TRIVALENT LANTHANIDES; CRYSTAL-STRUCTURE; ACTINIDES;
PLUTONIUM(III); ABSORPTION; EXTRACTION; PHOTOLUMINESCENCE
AB Advancing our understanding of the minor actinides (Am, Cm) versus lanthanides is key for developing advanced nuclear-fuel cycles. Herein, we describe the preparation of (NBu4)Am[S2P((Bu2C12H6)-Bu-t)](4) and two isomorphous lanthanide complexes, namely one with a similar ionic radius (i.e., Nd-III) and an isoelectronic one (Eu-III). The results include the first measurement of an Am-S bond length, with a mean value of 2.921(9)angstrom, by single-crystal X-ray diffraction. Comparison with the Eu-III and Nd-III complexes revealed subtle electronic differences between the complexes of Am-III and the lanthanides.
C1 [Cross, Justin N.; Macor, Joseph A.; Ferrier, Maryline G.; Kozimor, Stosh A.; Maassen, Joel R.; Scott, Brian L.; Stein, Benjamin W.; Stieber, S. Chantal E.] Los Alamos Natl Lab, Los Alamos, NM 87545 USA.
[Macor, Joseph A.; Bertke, Jeffery A.; Girolami, Gregory S.] Univ Illinois, Urbana, IL 61801 USA.
[Stieber, S. Chantal E.] Calif State Polytech Univ Pomona, Pomona, CA 91768 USA.
[Shuh, David K.] Lawrence Berkeley Natl Lab, Berkeley, CA 94720 USA.
RP Kozimor, SA (reprint author), Los Alamos Natl Lab, Los Alamos, NM 87545 USA.; Girolami, GS (reprint author), Univ Illinois, Urbana, IL 61801 USA.
EM ggirolam@illinois.edu; stosh@lanl.gov
RI Scott, Brian/D-8995-2017;
OI Scott, Brian/0000-0003-0468-5396; Cross, Justin/0000-0003-1881-155X
FU United States Department of Energy, Office of Science, Isotope
Development and Production for Research and Application Subprogram
within the Office of Nuclear Physics; Heavy Element Chemistry Program at
LANL by the Division of Chemical Sciences, Geosciences, and Biosciences,
Office of Basic Energy Sciences, U.S. Department of Energy; U.S.
Department of Energy [DE-AC52-06NA25396]; Office of Science, Office of
Basic Energy Sciences, Division of Chemical Sciences, Geosciences and
the Biosciences Heavy Element Chemistry Program of the U.S. Department
of Energy at Lawrence Berkeley National Laboratory [DE-AC02-05CH11231];
Glenn T. Seaborg Institute; National Science Foundation [CHE 13-62931]
FX We thank the United States Department of Energy, Office of Science,
Isotope Development and Production for Research and Application
Subprogram within the Office of Nuclear Physics for support and for
supplying the 243Am isotope used in these studies. Research
efforts were funded under the Heavy Element Chemistry Program at LANL by
the Division of Chemical Sciences, Geosciences, and Biosciences, Office
of Basic Energy Sciences, U.S. Department of Energy (S.A.K.). Los Alamos
National Laboratory is operated by Los Alamos National Security, LLC,
for the National Nuclear Security Administration of the U.S. Department
of Energy (DE-AC52-06NA25396). LBNL efforts (D.K.S.) were supported by
the Director, Office of Science, Office of Basic Energy Sciences,
Division of Chemical Sciences, Geosciences and the Biosciences Heavy
Element Chemistry Program of the U.S. Department of Energy at Lawrence
Berkeley National Laboratory (DE-AC02-05CH11231). We thank the Office of
Nuclear Energy Fuel Cycle R&D Program (J.A.M.). Some of this work was
also supported by Fellowships from the Glenn T. Seaborg Institute
(J.A.M., M.G.F., B.W.S., S.C.E.S.) and the Director's Postdoctoral
Fellowship (J.N.C.). Work at the University of Illinois was funded by
the National Science Foundation (CHE 13-62931, G.S.G.).
NR 57
TC 0
Z9 0
U1 16
U2 16
PU WILEY-V C H VERLAG GMBH
PI WEINHEIM
PA POSTFACH 101161, 69451 WEINHEIM, GERMANY
SN 1433-7851
EI 1521-3773
J9 ANGEW CHEM INT EDIT
JI Angew. Chem.-Int. Edit.
PD OCT 4
PY 2016
VL 55
IS 41
BP 12755
EP 12759
DI 10.1002/anie.201606367
PG 5
WC Chemistry, Multidisciplinary
SC Chemistry
GA DZ2ZU
UT WOS:000385713200030
PM 27629989
ER
PT J
AU Liu, ZM
Pan, HH
Zhu, GX
Li, YL
Tao, JH
Jin, B
Tang, RK
AF Liu, Zhaoming
Pan, Haihua
Zhu, Genxing
Li, Yaling
Tao, Jinhui
Jin, Biao
Tang, Ruikang
TI Realignment of Nanocrystal Aggregates into Single Crystals as a Result
of Inherent Surface Stress
SO ANGEWANDTE CHEMIE-INTERNATIONAL EDITION
LA English
DT Article
DE aggregation; calcium carbonate; crystal growth; crystal orientation;
surface stress
ID AMORPHOUS CALCIUM-CARBONATE; ORIENTED ATTACHMENT; GROWTH;
CRYSTALLIZATION; MESOCRYSTALS; PHOSPHATE; NUCLEATION; BONE;
TRANSFORMATION; ZEBRAFISH
AB Crystallization by particle attachment is widely observed in both natural and synthetic environments. Although this form of nonclassical crystallization is generally described by oriented attachment, random aggregation of building blocks to give single-crystal products is also observed, but the mechanism of crystallographic realignment is unknown. We herein reveal that random attachment during aggregation-based growth initially produces a nonoriented growth front. Subsequent evolution of the orientation is driven by the inherent surface stress applied by the disordered surface layer and results in single-crystal formation by grain-boundary migration. This mechanism is corroborated by measurements of orientation rate versus external stress, which demonstrated a predictive relationship between the two. These findings advance our understandings about aggregation-based growth via nanocrystal blocks and suggest an approach to material synthesis that takes advantage of stress-induced coalignment.
C1 [Liu, Zhaoming; Zhu, Genxing; Li, Yaling; Jin, Biao; Tang, Ruikang] Zhejiang Univ, Dept Chem, Hangzhou 310027, Zhejiang, Peoples R China.
[Pan, Haihua; Tang, Ruikang] Zhejiang Univ, Qiushi Acad Adv Studies, Hangzhou 310027, Zhejiang, Peoples R China.
[Tao, Jinhui] Pacific Northwest Natl Lab, Div Phys Sci, Richland, WA 99354 USA.
RP Tang, RK (reprint author), Zhejiang Univ, Dept Chem, Hangzhou 310027, Zhejiang, Peoples R China.; Pan, HH; Tang, RK (reprint author), Zhejiang Univ, Qiushi Acad Adv Studies, Hangzhou 310027, Zhejiang, Peoples R China.
EM panhh@zju.edu.cn; rtang@zju.edu.cn
FU Fundamental Research Funds for the Central Universities [2012XZZX005];
National Natural Science Foundation of China [21571155]; US Department
of Energy (DOE), Office of Basic Energy Sciences, Division of Chemical
Sciences, Geosciences, and Biosciences; US DOE [DE-AC05-76RL01830]
FX We thank James De Yoreo and Jennifer Soltis for helpful discussions. We
also thank Qiaohong He for TEM assistance. This research was supported
by the Fundamental Research Funds for the Central Universities
(2012XZZX005) and the National Natural Science Foundation of China (No.
21571155). The AFM measurements were supported by the US Department of
Energy (DOE), Office of Basic Energy Sciences, Division of Chemical
Sciences, Geosciences, and Biosciences and were performed at Pacific
Northwest National Laboratory, which is a multiprogram national
laboratory operated by Battelle for the US DOE under Contract
DE-AC05-76RL01830.
NR 32
TC 3
Z9 3
U1 31
U2 31
PU WILEY-V C H VERLAG GMBH
PI WEINHEIM
PA POSTFACH 101161, 69451 WEINHEIM, GERMANY
SN 1433-7851
EI 1521-3773
J9 ANGEW CHEM INT EDIT
JI Angew. Chem.-Int. Edit.
PD OCT 4
PY 2016
VL 55
IS 41
BP 12836
EP 12840
DI 10.1002/anie.201603794
PG 5
WC Chemistry, Multidisciplinary
SC Chemistry
GA DZ2ZU
UT WOS:000385713200047
PM 27430625
ER
PT J
AU Zhou, C
Penner, JE
Lin, GX
Liu, XH
Wang, MH
AF Zhou, Cheng
Penner, Joyce E.
Lin, Guangxing
Liu, Xiaohong
Wang, Minghuai
TI What controls the low ice number concentration in the upper troposphere?
SO ATMOSPHERIC CHEMISTRY AND PHYSICS
LA English
DT Article
ID COMMUNITY ATMOSPHERE MODEL; CIRRUS CLOUD FORMATION; TROPICAL TROPOPAUSE
LAYER; MESOSCALE TEMPERATURE-FLUCTUATIONS; NUCLEATION PARAMETERIZATIONS;
MICROPHYSICS SCHEME; BULK MICROPHYSICS; CRYSTAL NUMBERS; VERSION-3 CAM3;
AEROSOLS
AB Cirrus clouds in the tropical tropopause play a key role in regulating the moisture entering the stratosphere through their dehydrating effect. Low ice number concentrations (<200 L-1) and high supersaturations (150-160 %) have been observed in these clouds. Different mechanisms have been proposed to explain these low ice number concentrations, including the inhibition of homogeneous freezing by the deposition of water vapour onto pre-existing ice crystals, heterogeneous ice formation on glassy organic aerosol ice nuclei (IN), and limiting the formation of ice number from high-frequency gravity waves. In this study, we examined the effect from three different representations of updraft velocities, the effect from pre-existing ice crystals, the effect from different water vapour deposition coefficients (alpha = 0.1 or 1), and the effect of 0.1% of the total secondary organic aerosol (SOA) particles acting as IN. Model-simulated ice crystal numbers are compared against an aircraft observational dataset.
Including the effect from water vapour deposition on preexisting ice particles can effectively reduce simulated incloud ice number concentrations for all model setups. A larger water vapour deposition coefficient (alpha = 1) can also efficiently reduce ice number concentrations at temperatures below 205 K, but less so at higher temperatures. SOA acting as IN is most effective at reducing ice number concentrations when the effective updraft velocities are moderate (similar to 0.05-0.2 m s(-1)). However, the effects of including SOA as IN and using (alpha = 1) are diminished when the effect from pre-existing ice is included.
When a grid-resolved large-scale updraft velocity (<0.1 m s(-1)) is used, the ice nucleation parameterization with homogeneous freezing only or with both homogeneous freezing and heterogeneous nucleation is able to generate low ice number concentrations in good agreement with observations for temperatures below 205K as long as the pre-existing ice effect is included. For the moderate updraft velocity (similar to 0.05-0.2 m s(-1)), simulated ice number concentrations in good agreement with observations at temperatures below 205K can be achieved if effects from pre-existing ice, a larger water vapour deposition coefficient (alpha = 1), and SOA IN are all included. Using the sub-grid-scale turbulent kinetic energy (TKE)-based updraft velocity (similar to 0-2 m s(-1)) always overestimates the ice number concentrations at temperatures below 205 K but compares well with observations at temperatures above 205 K when the pre-existing ice effect is included.
C1 [Zhou, Cheng; Penner, Joyce E.; Lin, Guangxing] Univ Michigan, Dept Climate & Space Sci & Engn, Ann Arbor, MI 48109 USA.
[Liu, Xiaohong] Univ Wyoming, Dept Atmospher Sci, Laramie, WY 82071 USA.
[Wang, Minghuai] Nanjing Univ, Inst Climate & Global Change Res, Nanjing 210023, Jiangsu, Peoples R China.
[Wang, Minghuai] Nanjing Univ, Sch Atmospher Sci, Nanjing 210023, Jiangsu, Peoples R China.
[Wang, Minghuai] Collaborat Innovat Ctr Climate Change, Nanjing, Jiangsu, Peoples R China.
[Lin, Guangxing] Pacific Northwest Natl Lab, Richland, WA USA.
RP Zhou, C (reprint author), Univ Michigan, Dept Climate & Space Sci & Engn, Ann Arbor, MI 48109 USA.
EM zhouc@umich.edu
RI Liu, Xiaohong/E-9304-2011
OI Zhou, Cheng/0000-0001-9095-2846; Liu, Xiaohong/0000-0002-3994-5955
FU NSF [AGS-0946739, AGS-1540954]; National Science Foundation
FX We thank the two anonymous reviewers and the editor, who greatly helped
improve this work. This work was supported by the NSF under grants
AGS-0946739 and AGS-1540954. We acknowledge high-performance computing
support from Yellowstone (http://n2t.net/ark:/85065/d7wd3xhc) provided
by NCAR's Computational and Information Systems Laboratory and sponsored
by the National Science Foundation.
NR 67
TC 1
Z9 1
U1 10
U2 10
PU COPERNICUS GESELLSCHAFT MBH
PI GOTTINGEN
PA BAHNHOFSALLEE 1E, GOTTINGEN, 37081, GERMANY
SN 1680-7316
EI 1680-7324
J9 ATMOS CHEM PHYS
JI Atmos. Chem. Phys.
PD OCT 4
PY 2016
VL 16
IS 19
BP 12411
EP 12424
DI 10.5194/acp-16-12411-2016
PG 14
WC Meteorology & Atmospheric Sciences
SC Meteorology & Atmospheric Sciences
GA DY8SW
UT WOS:000385402200002
ER
PT J
AU Aaboud, M
Aad, G
Abbott, B
Abdallah, J
Abdinov, O
Abeloos, B
Aben, R
AbouZeid, OS
Abraham, NL
Abramowicz, H
Abreu, H
Abreu, R
Abulaiti, Y
Acharya, BS
Adachi, S
Adamczyk, L
Adams, DL
Adelman, J
Adomeit, S
Adye, T
Affolder, AA
Agatonovic-Jovin, T
Agricola, J
Aguilar-Saavedra, JA
Ahlen, SP
Ahmadov, F
Aielli, G
Akerstedt, H
Kesson, TPA
Akimov, AV
Alberghi, GL
Albert, J
Albrand, S
Verzini, MJA
Aleksa, M
Aleksandrov, IN
Alexa, C
Alexander, G
Alexopoulos, T
Alhroob, M
Ali, B
Aliev, M
Alimonti, G
Alison, J
Alkire, SP
Allbrooke, BMM
Allen, BW
Allport, PP
Aloisio, A
Alonso, A
Alonso, F
Alpigiani, C
Alshehri, AA
Alstaty, M
Gonzalez, BA
Piqueras, DA
Alviggi, MG
Amadio, BT
Amako, K
Coutinho, YA
Amelung, C
Amidei, D
Dos Santos, SPA
Amorim, A
Amoroso, S
Amundsen, G
Anastopoulos, C
Ancu, LS
Andari, N
Andeen, T
Anders, CF
Anders, G
Anders, JK
Anderson, KJ
Andreazza, A
Andrei, V
Angelidakis, S
Angelozzi, I
Anger, P
Angerami, A
Anghinolfi, F
Anisenkov, AV
Anjos, N
Annovi, A
Antel, C
Antonelli, M
Antonov, A
Anulli, F
Aoki, M
Bella, LA
Arabidze, G
Arai, Y
Araque, JP
Arce, ATH
Arduh, FA
Arguin, JF
Argyropoulos, S
Arik, M
Armbruster, AJ
Armitage, LJ
Arnaez, O
Arnold, H
Arratia, M
Arslan, O
Artamonov, A
Artoni, G
Artz, S
Asai, S
Asbah, N
Ashkenazi, A
Aring;sman, B
Asquith, L
Assamagan, K
Astalos, R
Atkinson, M
Atlay, NB
Augsten, K
Avolio, G
Axen, B
Ayoub, MK
Azuelos, G
Baak, MA
Baas, AE
Baca, MJ
Bachacou, H
Bachas, K
Backes, M
Backhaus, M
Bagiacchi, P
Bagnaia, P
Bai, Y
Baines, JT
Baker, OK
Baldin, EM
Balek, P
Balestri, T
Balli, F
Balunas, WK
Banas, E
Banerjee, S
Bannoura, AAE
Barak, L
Barberio, EL
Barberis, D
Barbero, M
Barillari, T
Barisits, MS
Barklow, T
Barlow, N
Barnes, SL
Barnett, BM
Barnett, RM
Barnovska-Blenessy, Z
Baroncelli, A
Barone, G
Barr, AJ
Navarro, LB
Barreiro, F
Da Costa, JBG
Bartoldus, R
Barton, AE
Bartos, P
Basalaev, A
Bassalat, A
Bates, RL
Batista, SJ
Batley, JR
Battaglia, M
Bauce, M
Bauer, F
Bawa, HS
Beacham, JB
Beattie, MD
Beau, T
Beauchemin, PH
Bechtle, P
Beck, HP
Becker, K
Becker, M
Beckingham, M
Becot, C
Beddall, AJ
Beddall, A
Bednyakov, VA
Bedognetti, M
Bee, CP
Beemster, LJ
Beermann, TA
Begel, M
Behr, JK
Belanger-Champagne, C
Bell, AS
Bella, G
Bellagamba, L
Bellerive, A
Bellomo, M
Belotskiy, K
Beltramello, O
Belyaev, NL
Benary, O
Benchekroun, D
Bender, M
Bendtz, K
Benekos, N
Benhammou, Y
Noccioli, EB
Benitez, J
Benjamin, DP
Bensinger, JR
Bentvelsen, S
Beresford, L
Beretta, M
Berge, D
Kuutmann, EB
Berger, N
Beringer, J
Berlendis, S
Bernard, NR
Bernius, C
Bernlochner, FU
Berry, T
Berta, P
Bertella, C
Bertoli, G
Bertolucci, F
Bertram, IA
Bertsche, C
Bertsche, D
Besjes, GJ
Bylund, OB
Bessner, M
Besson, N
Betancourt, C
Bethani, A
Bethke, S
Bevan, AJ
Bianchi, RM
Bianchini, L
Bianco, M
Biebel, O
Biedermann, D
Bielski, R
Biesuz, NV
Biglietti, M
De Mendizabal, JB
Billoud, TRV
Bilokon, H
Bindi, M
Binet, S
Bingul, A
Bini, C
Biondi, S
Bisanz, T
Bjergaard, DM
Black, CW
Black, JE
Black, KM
Blackburn, D
Blair, RE
Blanchard, JB
Blazek, T
Bloch, I
Blocker, C
Blue, A
Blum, W
Blumenschein, U
Blunier, S
Bobbink, GJ
Bobrovnikov, VS
Bocchetta, SS
Bocci, A
Bock, C
Boehler, M
Boerner, D
Bogaerts, JA
Bogavac, D
Bogdanchikov, AG
Bohm, C
Boisvert, V
Bokan, P
Bold, T
Boldyrev, AS
Bomben, M
Bona, M
Boonekamp, M
Borisov, A
Borissov, G
Bortfeldt, J
Bortoletto, D
Bortolotto, V
Bos, K
Boscherini, D
Bosman, M
Sola, JDB
Boudreau, J
Bouffard, J
Bouhova-Thacker, EV
Boumediene, D
Bourdarios, C
Boutle, SK
Boveia, A
Boyd, J
Boyko, IR
Bracinik, J
Brandt, A
Brandt, G
Brandt, O
Bratzler, U
Brau, B
Brau, JE
Madden, WDB
Brendlinger, K
Brennan, AJ
Brenner, L
Brenner, R
Bressler, S
Bristow, TM
Britton, D
Britzger, D
Brochu, FM
Brock, I
Brock, R
Brooijmans, G
Brooks, T
Brooks, WK
Brosamer, J
Brost, E
Broughton, JH
de Renstrom, PAB
Bruncko, D
Bruneliere, R
Bruni, A
Bruni, G
Bruni, LS
Brunt, B
Bruschi, M
Bruscino, N
Bryant, P
Bryngemark, L
Buanes, T
Buat, Q
Buchholz, P
Buckley, AG
Budagov, IA
Buehrer, F
Bugge, MK
Bulekov, O
Bullock, D
Burckhart, H
Burdin, S
Burgard, CD
Burghgrave, B
Burka, K
Burke, S
Burmeister, I
Burr, JTP
Busato, E
Buscher, D
Buscher, V
Bussey, P
Butler, JM
Buttar, CM
Butterworth, JM
Butti, P
Buttinger, W
Buzatu, A
Buzykaev, AR
Urban, SC
Caforio, D
Cairo, VM
Cakir, O
Calace, N
Calafiura, P
Calandri, A
Calderini, G
Calfayan, P
Callea, G
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Yusuff, I.
Zabinski, B.
Zaidan, R.
Zaitsev, A. M.
Zakharchuk, N.
Zalieckas, J.
Zaman, A.
Zambito, S.
Zanello, L.
Zanzi, D.
Zeitnitz, C.
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Zemla, A.
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Zenis, T.
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Zhu, J.
Zhu, Y.
Zhuang, X.
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Zieminska, D.
Zimine, N. I.
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Zivkovic, L.
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Zoccoli, A.
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Zwalinski, L.
CA ATLAS Collaboration
TI Search for new phenomena in different-flavour high-mass dilepton final
states in pp collisions at root s=13Tev with the ATLAS detector
SO EUROPEAN PHYSICAL JOURNAL C
LA English
DT Article
ID DIMENSIONS; LHC; SUPERSYMMETRY; HIERARCHY; EXTENSION; DECAY
AB A search is performed for a heavy particle decaying into different flavour dilepton pairs (, or ), using 3.2 fb of proton-proton collision data at TeV collected in 2015 by the ATLAS detector at the Large Hadron Collider. No excess over the Standard Model prediction is observed. Limits at the 95 % credibility level are set on the mass of a boson with lepton-flavour-violating couplings at 3.0, 2.7 and 2.6 TeV, and on the mass of a supersymmetric sneutrino with R-parity-violating couplings at 2.3, 2.2 and 1.9 TeV, for , and final states, respectively. The results are also interpreted as limits on the threshold mass for quantum black hole production.
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[Blunier, S.; Diaz, M. A.; Ochoa-Ricoux, J. P.] Pontificia Univ Catolica Chile, Dept Fis, Santiago, Chile.
[Brooks, W. K.; Carquin, E.; Kuleshov, S.; Lpez, J. A.; Pezoa, R.; Prokoshin, F.; Loyola, J. E. Salazar; Araya, S. Tapia; Vasquez, G. A.; White, R.] Univ Tecn Federico Santa Maria, Dept Fis, Valparaiso, Chile.
[Bai, Y.; da Costa, J. Barreiro Guimares; Cheng, H. J.; Fang, Y.; Jin, S.; Li, Q.; Liang, Z.; Merino, J. Llorente; Lou, X.; Mansour, J. D.; Ouyang, Q.; Peng, C.; Ren, H.; Shan, L. Y.; Sun, X.; Xu, D.; Zhu, H.; Zhuang, X.] Chinese Acad Sci, Inst High Energy Phys, Beijing, Peoples R China.
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INFN, Lab Nazl Frascati, Grp Coll Cosenza, Frascati, Italy.
[Cairo, V. M.; Callea, G.; Capua, M.; Crosetti, G.; Del Gaudio, M.; La Rotonda, L.; Mastroberardino, A.; Palazzo, S.; Policicchio, A.; Salvatore, D.; Scarfone, V.; Schioppa, M.; Susinno, G.; Tassi, E.] Univ Calabria, Dipartimento Fis, Arcavacata Di Rende, Italy.
[Adamczyk, L.; Bold, T.; Dabrowski, W.; Gach, G. P.; Grabowska-Bold, I.; Kisielewska, D.; Koperny, S.; Kowalski, T. Z.; Mindur, B.; Przybycien, M.; Zemla, A.] AGH Univ Sci & Technol, Fac Phys & Appl Comp Sci, Krakow, Poland.
[Palka, M.; Richter-Was, E.] Jagiellonian Univ, Marian Smoluchowski Inst Phys, Krakow, Poland.
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[Burmeister, I.; Cinca, D.; Dette, K.; Erdmann, J.; Esch, H.; Gossling, C.; Homann, M.; Klingenberg, R.; Kroeninger, K.] Tech Univ Dortmund, Lehrstuhl Expt Phys 4, Dortmund, Germany.
[Anger, P.; Duschinger, D.; Friedrich, F.; Grohs, J. P.; Gutschow, C.; Hauswald, L.; Kobel, M.; Mader, W. F.; Novgorodova, O.; Siegert, F.; Socher, F.; Straessner, A.; Vest, A.; Wahrmund, S.] Tech Univ Dresden, Inst Kern & Teilchenphys, Dresden, Germany.
[Arce, A. T. H.; Benjamin, D. P.; Bjergaard, D. M.; Bocci, A.; Cerio, B. C.; Goshaw, A. T.; Kajomovitz, E.; Kotwal, A.; Kruse, M. C.; Li, L.; Li, S.; Liu, M.; Oh, S. H.] Duke Univ, Dept Phys, Durham, NC 27706 USA.
[Bristow, T. M.; Clark, P. J.; Dias, F. A.; Edwards, N. C.; Gao, Y.; Walls, F. M. Garay; Glaysher, P. C. F.; Harrington, R. D.; Leonidopoulos, C.; Martin, V. J.; MijoviAO, L.; Mills, C.; Pino, S. A. Olivares; Washbrook, A.; Wynne, B. M.] Univ Edinburgh, SUPA Sch Phys & Astron, Edinburgh, Midlothian, Scotland.
[Antonelli, M.; Beretta, M.; Bilokon, H.; Chiarella, V.; Curatolo, M.; Esposito, B.; Gatti, C.; Laurelli, P.; Maccarrone, G.; Mancini, G.; Sansoni, A.; Testa, M.; Vilucchi, E.] INFN, Lab Nazl Frascati, Frascati, Italy.
[Arnold, H.; Betancourt, C.; Boehler, M.; Bruneliere, R.; Buehrer, F.; Burgard, C. D.; Buscher, D.; Cardillo, F.; Coniavitis, E.; Consorti, V.; Dang, N. P.; Dao, V.; Di Simone, A.; Glatzer, J.; Gonella, G.; Herten, G.; Hirose, M.; Jakobs, K.; Javurek, T.; Jenni, P.; Kiss, F.; Koneke, K.; Kopp, A. K.; Kuehn, S.; Landgraf, U.; Luedtke, C.; Nagel, M.; Pagaova, M.; Parzefall, U.; Ronzani, M.; Rosbach, K.; Ruhr, F.; Rurikova, Z.; Sammel, D.; Schillo, C.; Schnoor, U.; Schumacher, M.; Sommer, P.; Sundermann, J. E.; Ta, D.; Temming, K. K.; Tornambe, P.; Tsiskaridze, V.; Weiser, C.; Werner, M.; Zhang, L.; Zimmermann, S.] Univ Freiburg, Fak Math & Phys, Freiburg, Germany.
[Ancu, L. S.; De Mendizabal, J. Bilbao; Calace, N.; Chatterjee, A.; Clark, A.; Coccaro, A.; Delitzsch, C. M.; della Volpe, D.; Ferrere, D.; Golling, T.; Gonzalez-Sevilla, S.; Gramling, J.; Guescini, F.; Iacobucci, G.; Katre, A.; Khoo, T. J.; Lanfermann, M. C.; Lionti, A. E.; March, L.; Mermod, P.; Nackenhorst, O.; Paolozzi, L.; RistiAO, B.; Schramm, S.; Sfyrla, A.; Wu, X.] Univ Geneva, Sect Phys, Geneva, Switzerland.
[Darbo, G.; Gemme, C.; Morettini, P.; Passaggio, S.; Rossi, L. P.] INFN, Sez Genova, Genoa, Italy.
[Barberis, D.; Favareto, A.; Parodi, A. Ferretto; Gagliardi, G.; Gaudiello, A.; Guido, E.; Miglioranzi, S.; Parodi, F.; Sannino, M.; Schiavi, C.] Univ Genoa, Dipartimento Fis, Genoa, Italy.
[Tskhadadze, E. G.] Iv Javakhishvili Tbilisi State Univ, Andronikashvili Inst Phys, Tbilisi, Rep of Georgia.
[Djobava, T.; Durglishvili, A.; Khubua, J.; Mosidze, M.] Tbilisi State Univ, Inst High Energy Phys, Tbilisi, Rep of Georgia.
[Duren, M.; Heinz, C.; Kreutzfeldt, K.; Stenzel, H.] Univ Giessen, Inst Phys 2, Giessen, Germany.
[Alshehri, A. A.; Bates, R. L.; Blue, A.; Boutle, S. K.; Madden, W. D. Breaden; Britton, D.; Buckley, A. G.; Bussey, P.; Buttar, C. M.; Buzatu, A.; Crawley, S. J.; D'Auria, S.; Doyle, A. T.; Gul, U.; Knue, A.; Mullen, P.; O'Shea, V.; Owen, M.; Pollard, C. S.; Qin, G.; Quilty, D.; Ravenscroft, T.; Robson, A.; Denis, R. D. St.; Stewart, G. A.; Thompson, A. S.] Univ Glasgow, SUPA Sch Phys & Astron, Glasgow, Lanark, Scotland.
[Agricola, J.; Bindi, M.; Bisanz, T.; Blumenschein, U.; Brandt, G.; De Maria, A.; Drechsler, E.; Graber, L.; Grosse-Knetter, J.; Janus, M.; Kareem, M. J.; Kawamura, G.; Lai, S.; Lemmer, B.; Magradze, E.; Mantoani, M.; Mchedlidze, G.; Llacer, M. Moreno; Musheghyan, H.; Quadt, A.; Rieger, J.; Rosien, N. -A.; Rzehorz, G. F.; Shabalina, E.; Stolte, P.; Veatch, J.; Weingarten, J.; Zinonos, Z.] Univ Gottingen, Inst Phys 2, Gottingen, Germany.
[Albrand, S.; Berlendis, S.; Bethani, A.; Camincher, C.; Collot, J.; Crepe-Renaudin, S.; Delsart, P. A.; Gabaldon, C.; Genest, M. H.; Gradin, P. O. J.; Hostachy, J-Y.; Ledroit-Guillon, F.; Lleres, A.; Lucotte, A.; Malek, F.; Petit, E.; Stark, J.; Trocme, B.; Wu, M.] Grenoble Alpes Univ, Lab Phys Subatom & Cosmol, Grenoble, France.
[Chan, S. K.; Clark, B. L.; Franklin, M.; Giromini, P.; Huth, J.; Ippolito, V.; Lazovich, T.; Mateos, D. Lopez; Morii, M.; Rogan, C. S.; Skottowe, H. P.; Sun, S.; Tolley, E.; Tong, B.; Tuna, A. N.; Yen, A. L.; Zambito, S.] Harvard Univ, Lab Particle Phys & Cosmol, Cambridge, MA 02138 USA.
[Gao, J.; Geng, C.; Guo, Y.; Han, L.; Hu, Q.; Jiang, Y.; Li, B.; Li, C.; Li, Q.; Liu, J. B.; Liu, M.; Liu, Y. L.; Liu, Y.; Peng, H.; Song, H. Y.; Wang, W.; Zhang, G.; Zhang, R.; Zhao, Z.; Zhu, Y.] Univ Sci & Technol China, Dept Modern Phys, Hefei 230026, Anhui, Peoples R China.
[Andrei, V.; Antel, C.; Baas, A. E.; Brandt, O.; Djuvsland, J. I.; Dunford, M.; Geisler, M. P.; Hanke, P.; Jongmanns, J.; Kluge, E. -E.; Lang, V. S.; Meier, K.; Theenhausen, H. Meyer Zu; Villar, D. I. Narrias; Sahinsoy, M.; Scharf, V.; Schultz-Coulon, H. -C.; Stamen, R.; Starovoitov, P.; Suchek, S.; Wessels, M.] Heidelberg Univ, Kirchhoff Inst Phys, Heidelberg, Germany.
[Anders, C. F.; de Lima, D. E. Ferreira; Giulini, M.; Kolb, M.; Lisovyi, M.; Schaetzel, S.; Schoening, A.; Sosa, D.] Heidelberg Univ, Inst Phys, Heidelberg, Germany.
[Kretz, M.; Kugel, A.] Heidelberg Univ, ZITI Inst Tech Informat, Mannheim, Germany.
[Nagasaka, Y.] Hiroshima Inst Technol, Fac Appl Informat Sci, Hiroshima, Japan.
[Chan, Y. L.; Castillo, L. R. Flores; Lu, H.; Tsui, K. M.] Chinese Univ Hong Kong, Dept Phys, Shatin, Hong Kong, Peoples R China.
[Orlando, N.; Tu, Y.] Univ Hong Kong, Dept Phys, Hong Kong, Peoples R China.
[Bortolotto, V.; Prokofiev, K.; Salvucci, A.] Hong Kong Univ Sci & Technol, Dept Phys, Kowloon, Hong Kong, Peoples R China.
[Choi, K.; Evans, H.; Gagnon, P.; Kopeliansky, R.; Lammers, S.; Martinez, N. Lorenzo; Luehring, F.; Ogren, H.; Penwell, J.; Weinert, B.; Zieminska, D.] Indiana Univ, Dept Phys, Bloomington, IN 47405 USA.
[Guenther, J.; Iwanski, W.; Jansky, R.; Kneringer, E.; Lukas, W.; Milic, A.] Univ Innsbruck, Inst Astro & Teilchenphys, Innsbruck, Austria.
[Abdallah, J.; Argyropoulos, S.; Benitez, J.; Mallik, U.; Zaidan, R.] Univ Iowa, Iowa City, IA USA.
[Chen, C.; Cochran, J.; De Lorenzi, F.; Jiang, H.; Krumnack, N.; Pluth, D.; Prell, S.; Werner, M. D.; Yu, J.] Iowa State Univ, Dept Phys & Astron, Ames, IA USA.
[Ahmadov, F.; Aleksandrov, I. N.; Bednyakov, V. A.; Boyko, I. R.; Budagov, I. A.; Chelkov, G. A.; Cheplakov, A.; Chizhov, M. V.; Dedovich, D. V.; Demichev, M.; Gongadze, A.; Gostkin, M. I.; Huseynov, N.; Javadov, N.; Karpov, S. N.; Karpova, Z. M.; Khramov, E.; Kruchonak, U.; Kukhtin, V.; Ladygin, E.; Lyubushkin, V.; Minashvili, I. A.; Mineev, M.; Peshekhonov, V. D.; Plotnikova, E.; Potrap, I. N.; Pozdnyakov, V.; Rusakovich, N. A.; Sadykov, R.; Sapronov, A.; Shiyakova, M.; Soloshenko, A.; Turchikhin, S.; Vinogradov, V. B.; Yeletskikh, I.; Zhemchugov, A.; Zimine, N. I.] JINR Dubna, Joint Inst Nucl Res, Dubna, Russia.
[Amako, K.; Aoki, M.; Arai, Y.; Hanagaki, K.; Honda, T.; Ikegami, Y.; Ikeno, M.; Iwasaki, H.; Kanzaki, J.; Kondo, T.; Kono, T.; Makida, Y.; Nagai, R.; Nagano, K.; Nakamura, K.; Nozaki, M.; Odaka, S.; Okuyama, T.; Sasaki, O.; Suzuki, S.; Takubo, Y.; Tanaka, S.; Terada, S.; Tokushuku, K.; Tsuno, S.; Unno, Y.; Yamamoto, A.; Yasu, Y.] KEK, High Energy Accelerator Res Org, Tsukuba, Ibaraki, Japan.
[Chen, Y.; Hasegawa, M.; Kido, S.; Kurashige, H.; Maeda, J.; Ochi, A.; Shimizu, S.; Tanioka, R.; Yamazaki, Y.; Yuan, L.] Kobe Univ, Grad Sch Sci, Kobe, Hyogo, Japan.
[Kunigo, T.; Monden, R.; Sumida, T.; Tashiro, T.] Kyoto Univ, Fac Sci, Kyoto, Japan.
[Takashima, R.] Kyoto Univ, Kyoto, Japan.
[Kawagoe, K.; Oda, S.; Otono, H.; Shirabe, S.; Tojo, J.] Kyushu Univ, Dept Phys, Fukuoka, Japan.
[Verzini, M. J. Alconada; Alonso, F.; Arduh, F. A.; Dova, M. T.; Hoya, J.; Monticelli, F.; Wahlberg, H.] Univ Nacl Plata, Inst Fis Plata, CONICET, La Plata, Buenos Aires, Argentina.
[Barton, A. E.; Beattie, M. D.; Bertram, I. A.; Borissov, G.; Bouhova-Thacker, E. V.; Dearnaley, W. J.; Fox, H.; Grimm, K.; Henderson, R. C. W.; Hughes, G.; Jones, R. W. L.; Kartvelishvili, V.; Long, R. E.; Love, P. A.; Muenstermann, D.; Parker, A. J.; Skinner, M. B.; Smizanska, M.; Walder, J.; Wharton, A. M.] Univ Lancaster, Dept Phys, Lancaster, England.
[Chiodini, G.; Primavera, M.] INFN, Sez Lecce, Lecce, Italy.
[Aliev, M.; Bachas, K.; Gorini, E.; Longo, L.; Reale, M.; Spagnolo, S.; Ventura, A.] Univ Salento, Dipartimento Matemat Fis, Lecce, Italy.
[Affolder, A. A.; Anders, J. K.; Burdin, S.; D'Onofrio, M.; Dervan, P.; Gwilliam, C. B.; Hayward, H. S.; Jones, T. J.; King, B. T.; Klein, M.; Klein, U.; Kretzschmar, J.; Laycock, P.; Lehan, A.; Maxfield, S. J.; Mehta, A.; Readioff, N. P.; Vossebeld, J. H.] Univ Liverpool, Oliver Lodge Lab, Liverpool, Merseyside, England.
[Cindro, V.; Filipi, A.; Goriek, A.; Kanjir, L.; Kerevan, B. P.; Kramberger, G.; Maek, B.; Mandic, I.; Mikuz, M.; Mukinja, M.; Sfiligoj, T.; Sokhrannyi, G.] Univ Ljubljana, Dept Phys, Ljubljana, Slovenia.
[Armitage, L. J.; Bevan, A. J.; Bona, M.; Hays, J. M.; Hickling, R.; Landon, M. P. J.; Lewis, D.; Lloyd, S. L.; Morris, J. D.; Nooney, T.; Piccaro, E.; Rizvi, E.; Sandbach, R. L.] Queen Mary Univ London, Sch Phys & Astron, London, England.
[Berry, T.; Boisvert, V.; Brooks, T.; Connelly, I. A.; Cowan, G.; Giannelli, M. Faucci; Gadomski, S.; George, S.; Gibson, S. M.; Kempster, J. J.; Kilby, C. R.; Vazquez, J. G. Panduro; Pastore, Fr.; Savage, G.; Sowden, B. C.; Span, F.; Teixeira-Dias, P.; Thomas-Wilsker, J.] Royal Holloway Univ London, Dept Phys, Surrey, England.
[Bell, A. S.; Butterworth, J. M.; Campanelli, M.; Christodoulou, V.; Cooper, B. D.; Davison, P.; Falla, R. J.; Freeborn, D.; Gregersen, K.; Grout, Z. J.; Ortiz, N. G. Gutierrez; Hesketh, G. G.; Jiggins, S.; Konstantinidis, N.; Korn, A.; Kucuk, H.; Leney, K. J. C.; Martyniuk, A. C.; McClymont, L. I.; Mcfayden, J. A.; Nurse, E.; Richter, S.; Scanlon, T.; Sherwood, P.; Simmons, B.; Wardrope, D. R.; Waugh, B. M.] UCL, Dept Phys & Astron, London, England.
[Greenwood, Z. D.; Grossi, G. C.; Jana, D. K.; Sawyer, L.] Louisiana Tech Univ, Ruston, LA 71270 USA.
[Beau, T.; Bomben, M.; Calderini, G.; Crescioli, F.; De Cecco, S.; Demilly, A.; Derue, F.; Francavilla, P.; Krasny, M. W.; Lacour, D.; Laforge, B.; Laplace, S.; Le Dortz, O.; Lefebvre, G.; Solis, A. Lopez; Luzi, P. M.; Malaescu, B.; Marchiori, G.; Nikolic-Audit, I.; Ocariz, J.; Pandini, C. E.; Pires, S.; Ridel, M.; Roos, L.; Trincaz-Duvoid, S.; Varouchas, D.; Yap, Y. C.] Univ Paris 06, CNRS, Lab Phys Nucl, INSERM, Paris, France.
[kesson, T. P. A.; Bocchetta, S. S.; Bryngemark, L.; Doglioni, C.; Hedberg, V.; Jarlskog, G.; Lytken, E.; Mjornmark, J. U.; Smirnova, O.; Viazlo, O.] Lund Univ, Fys Inst, Lund, Sweden.
[Barreiro, F.; Lopez, S. Calvente; Cueto, A.; Del Peso, J.; Glasman, C.; Terron, J.] Univ Autonoma Madrid, Dept Fis Teor, Madrid, Spain.
[Artz, S.; Becker, M.; Bertella, C.; Blum, W.; Buscher, V.; Dudder, A. Chr.; Endner, O. C.; Ertel, E.; Fiedler, F.; Torregrosa, E. Fullana; Geisen, M.; Groh, S.; Heck, T.; Jakobi, K. B.; Kaluza, A.; Karnevskiy, M.; Kleinknecht, K.; Kopke, L.; Lin, T. H.; Masetti, L.; Mattmann, J.; Meyer, C.; Moritz, S.; Pleskot, V.; Rave, S.; Reiss, A.; Sander, H. G.; Schaeffer, J.; Schafer, U.; Schmitt, C.; Schmitz, S.; Schott, M.; Schuh, N.; Schulte, A.; Simioni, E.; Simon, M.; Tapprogge, S.; Urrejola, P.; Webb, S.; Yildirim, E.; Zimmermann, C.; Zinser, M.] Johannes Gutenberg Univ Mainz, Inst Phys, Mainz, Germany.
[Barnes, S. L.; Bielski, R.; Cox, B. E.; Da Via, C.; Dann, N. S.; Forcolin, G. T.; Forti, A.; Ponce, J. M. Iturbe; Li, X.; Loebinger, F. K.; Marsden, S. P.; Masik, J.; Sanchez, F. J. Munoz; Neep, T. J.; Oh, A.; Ospanov, R.; Pater, J. R.; Peters, R. F. Y.; Pilkington, A. D.; Pin, A. W. J.; Price, D.; Qin, Y.; Queitsch-Maitland, M.; Raine, J. A.; Schweiger, H.; Shaw, S. M.; Tomlinson, L.; Watts, S.; Wilk, F.; Woudstra, M. J.; Wyatt, T. R.] Univ Manchester, Sch Phys & Astron, Manchester, Lancs, England.
[Aad, G.; Alstaty, M.; Barbero, M.; Calandri, A.; Calvet, T. P.; Coadou, Y.; Diaconu, C.; Djama, F.; Ellajosyula, V.; Feligioni, L.; Hadef, A.; Hallewell, G. D.; Hubaut, F.; Kahn, S. J.; Knoops, E. B. F. G.; Le Guirriec, E.; Liu, J.; Liu, K.; Madaffari, D.; Monnier, E.; Muanza, S.; Nagy, E.; Pralavorio, P.; Rodina, Y.; Rozanov, A.; Talby, M.; Theveneaux-Pelzer, T.; Torres, R. E. Ticse; Tisserant, S.; Toth, J.; Touchard, F.; Vacavant, L.] Aix Marseille Univ, CPPM, CNRS, IN2P3, Marseille, France.
[Bellomo, M.; Bernard, N. R.; Brau, B.; Dallapiccola, C.; Moyse, E. J. W.; Pais, P.; Pettersson, N. E.; Picazio, A.; Willocq, S.] Univ Massachusetts, Dept Phys, Amherst, MA USA.
[Belanger-Champagne, C.; Chuinard, A. J.; Corriveau, F.; Keyes, R. A.; Lefebvre, B.; Mantifel, R.; Prince, S.; Robertson, S. H.; Robichaud-Veronneau, A.; Stockton, M. C.; Stoebe, M.; Vachon, B.; Schroeder, T. Vazquez; Wang, K.; Warburton, A.] McGill Univ, Dept Phys, Montreal, PQ, Canada.
[Barberio, E. L.; Brennan, A. J.; Dawe, E.; Goldfarb, S.; Jennens, D.; Kubota, T.; Le, B.; McDonald, E. F.; Milesi, M.; Nuti, F.; Rados, P.; Scutti, F.; Spiller, L. A.; Tan, K. G.; Taylor, G. N.; Taylor, P. T. E.; Ungaro, F. C.; Urquijo, P.; Volpi, M.; Zanzi, D.] Univ Melbourne, Sch Phys, Melbourne, Vic, Australia.
[Amidei, D.; Chelstowska, M. A.; Cheng, H. C.; Dai, T.; Diehl, E. B.; Edgar, R. C.; Feng, H.; Ferretti, C.; Fleischmann, P.; Guan, L.; Levin, D.; Liu, H.; Lu, N.; Marley, D. E.; Mc Kee, S. P.; McCarn, A.; Neal, H. A.; Qian, J.; Schwarz, T. A.; Searcy, J.; Sekhon, K.; Wu, Y.; Yu, J. M.; Zhang, D.; Zhou, B.; Zhu, J.] Univ Michigan, Dept Phys, Ann Arbor, MI 48109 USA.
[Arabidze, G.; Brock, R.; Chegwidden, A.; De la Torre, H.; Fisher, W. C.; Halladjian, G.; Hauser, R.; Hayden, D.; Huston, J.; Martin, B.; Mondragon, M. C.; Plucinski, P.; Pope, B. G.; Schoenrock, B. D.; Schwienhorst, R.; Willis, C.] Michigan State Univ, Dept Phys & Astron, E Lansing, MI 48824 USA.
[Alimonti, G.; Cavalli, D.; Citterio, M.; Costa, G.; Giugni, D.; Lari, T.; Mandelli, L.; Meroni, C.; Resconi, S.; Stabile, A.; Tartarelli, G. F.; Troncon, C.] INFN, Sez Milano, Milan, Italy.
[Andreazza, A.; Camplani, A.; Carminati, L.; Fanti, M.; Lazzaroni, M.; Manzoni, S.; Mazza, S. M.; Monzani, S.; Perini, L.; Ragusa, F.; Ratti, M. G.; Shojaii, S.; Turra, R.; Perez, M. Villaplana] Univ Milan, Dipartimento Fis, Milan, Italy.
[Harkusha, S.; Kulchitsky, Y.; Kurochkin, Y. A.; Tsiareshka, P. V.] Natl Acad Sci Belarus, B Stepanov Inst Phys, Minsk, Byelarus.
[Hrynevich, A.] Natl Sci & Educ Ctr Particle & High Energy Phys, Minsk, Byelarus.
[Arguin, J-F.; Azuelos, G.; Billoud, T. R. V.; Dallaire, F.; Ducu, O. A.; Gagnon, L. G.; Gauthier, L.; Leroy, C.; Mochizuki, K.; Manh, T. Nguyen; Rezvani, R.; Saadi, D. Shoaleh] Univ Montreal, Grp Particle Phys, Montreal, PQ, Canada.
[Akimov, A. V.; Gavrilenko, I. L.; Komar, A. A.; Mashinistov, R.; Nechaeva, P. Yu.; Shmeleva, A.; Snesarev, A. A.; Sulin, V. V.; Tikhomirov, V. O.; Zhukov, K.] Russian Acad Sci, PN Lebedev Phys Inst, Moscow, Russia.
[Artamonov, A.; Gorbounov, P. A.; Khovanskiy, V.; Shatalov, P. B.; Tsukerman, I. I.] ITEP, Moscow, Russia.
[Antonov, A.; Belotskiy, K.; Belyaev, N. L.; Bulekov, O.; Kantserov, V. A.; Krasnopevtsev, D.; Romaniouk, A.; Shulga, E.; Smirnov, S. Yu.; Smirnov, Y.; Soldatov, E. Yu.; Timoshenko, S.; Vorobev, K.] Natl Res Nucl Univ MEPhI, Moscow, Russia.
[Gladilin, L. K.; Kramarenko, V. A.; Maevskiy, A.; Sivoklokov, S. Yu.; Smirnova, L. N.] M Lomonosov Moscow State Univ, Skobeltsyn Inst Nucl Phys, Moscow, Russia.
[Adomeit, S.; Bender, M.; Biebel, O.; Bock, C.; Calfayan, P.; Chow, B. K. B.; Duckeck, G.; Hartmann, N. M.; Heinrich, J. J.; Hertenberger, R.; Hoenig, F.; Legger, F.; Lorenz, J.; Losel, P. J.; Maier, T.; Mann, A.; Mehlhase, S.; Meineck, C.; Mitrevski, J.; Mueller, R. S. P.; Rauscher, F.; Ruschke, A.; Schachtner, B. M.; Schaile, D.; Unverdorben, C.; Valderanis, C.; Walker, R.; Wittkowski, J.] Univ Munich, Fak Phys, Munich, Germany.
[Barillari, T.; Bethke, S.; Compostella, G.; Cortiana, G.; Ecker, K. M.; Flowerdew, M. J.; Giuliani, C.; Ince, T.; Kiryunin, A. E.; Kluth, S.; Koehler, N. M.; Kortner, O.; Kortner, S.; Kroha, H.; La Rosa, A.; Macchiolo, A.; Maier, A. A.; McCarthy, T. G.; Menke, S.; Mueller, F.; Nisius, R.; Nowak, S.; Oberlack, H.; Richter, R.; Salihagic, D.; Savic, N.; Schacht, P.; Schmidt-Sommerfeld, K. R.; Spettel, F.; Stonjek, S.; von der Schmitt, H.; Wildauer, A.] Max Planck Inst Phys & Astrophys, Werner Heisenberg Inst, Munich, Germany.
[Fusayasu, T.; Shimojima, M.] Nagasaki Inst Appl Sci, Nagasaki, Japan.
[Horii, Y.; Kawade, K.; Nakahama, Y.; Onogi, K.; Tomoto, M.; Wakabayashi, J.; Yamauchi, K.] Nagoya Univ, Grad Sch Sci, Kobayashi Maskawa Inst, Nagoya, Aichi, Japan.
[Carlino, G.; Conventi, F.; de Asmundis, R.; Della Pietra, M.; Doria, A.; Izzo, V.; Sekhniaidze, G.] INFN, Sez Napoli, Naples, Italy.
[Aloisio, A.; Alviggi, M. G.; Canale, V.; Cirotto, F.; Merola, L.; Perrella, S.; Rossi, E.; Sanchez, A.] Univ Napoli, Dipartimento Fis, Naples, Italy.
[Gorelov, I.; Hoeferkamp, M. R.; Mc Fadden, N. C.; Seidel, S. C.; Taylor, A. C.; Toms, K.] Univ New Mexico, Dept Phys & Astron, Albuquerque, NM 87131 USA.
[Caron, S.; Colasurdo, L.; Croft, V.; De Groot, N.; Filthaut, F.; Galea, C.; Konig, A. C.; Nektarijevic, S.; Schouwenberg, J. F. P.; Strubig, A.] Radboud Univ Nijmegen, Inst Math Astrophys & Particle Phys, Nijmegen, Netherlands.
[Aben, R.; Angelozzi, I.; Bedognetti, M.; Beemster, L. J.; Bentvelsen, S.; Berge, D.; Bobbink, G. J.; Bos, K.; Brenner, L.; Bruni, L. S.; Butti, P.; Castelijn, R.; Castelli, A.; Colijn, A. P.; de Jong, P.; Deigaard, I.; Duda, D.; Ferrari, P.; Hartjes, F.; Hessey, N. P.; Igonkina, O.; Kluit, P.; Koffeman, E.; Mahlstedt, J.; Meyer, J.; Oussoren, K. P.; Sabato, G.; Salek, D.; Slawinska, M.; Valencic, N.; Van den Wollenberg, W.; Van der Deijl, P. C.; van der Graaf, H.; van Vulpen, I.; Vankov, P.; Verkerke, W.; Vermeulen, J. C.; Vreeswijk, M.; Weits, H.; Williams, S.; Wolf, T. M. H.] Univ Amsterdam, Nikhef Natl Inst Subat Phys, Amsterdam, Netherlands.
[Adelman, J.; Brost, E.; Burghgrave, B.; Chakraborty, D.; Klimek, P.; Saha, P.] Univ Illinois, Dept Phys, De Kalb, IL USA.
[Anisenkov, A. V.; Baldin, E. M.; Bobrovnikov, V. S.; Bogdanchikov, A. G.; Buzykaev, A. R.; Kazanin, V. F.; Kharlamov, A. G.; Kharlamova, T.; Korol, A. A.; Maslennikov, A. L.; Maximov, D. A.; Peleganchuk, S. V.; Rezanova, O. L.; Soukharev, A. M.; Talyshev, A. A.; Tikhonov, Yu. A.] RAS, Budker Inst Nucl Phys, SB, Novosibirsk, Russia.
[Becot, C.; Bernius, C.; Cranmer, K.; Haas, A.; Heinrich, L.; Kaplan, B.; Karthik, K.; Konoplich, R.; Mincer, A. I.; Nemethy, P.; Neves, R. M.] NYU, Dept Phys, 4 Washington Pl, New York, NY 10003 USA.
[Beacham, J. B.; Che, S.; Gan, K. K.; Ishmukhametov, R.; Kagan, H.; Kass, R. D.; Looper, K. A.; Shrestha, S.; Tannenwald, B. B.] Ohio State Univ, Columbus, OH 43210 USA.
[Nakano, I.] Okayama Univ, Fac Sci, Okayama, Japan.
[Abbott, B.; Alhroob, M.; Bertsche, D.; De Benedetti, A.; Gutierrez, P.; Hasib, A.; Norberg, S.; Pearson, B.; Rifki, O.; Severini, H.; Shope, D. R.; Skubic, P.; Strauss, M.] Univ Oklahoma, Homer L Dodge Dept Phys & Astron, Norman, OK USA.
[Cantero, J.; Haley, J.; Jamin, D. O.; Khanov, A.; Rizatdinova, F.; Sidorov, D.] Oklahoma State Univ, Dept Phys, Stillwater, OK 74078 USA.
[Chytka, L.; Hamal, P.; Hrabovsky, M.; Kvita, J.; Nozka, L.] Palacky Univ, RCPTM, Olomouc, Czech Republic.
[Abreu, R.; Allen, B. W.; Brau, J. E.; Dattagupta, A.; Hopkins, W. H.; Majewski, S.; Potter, C. T.; Radloff, P.; Sinev, N. B.; Snyder, I. M.; Strom, D. M.; Torrence, E.; Wanotayaroj, C.; Whalen, K.; Winklmeier, F.] Univ Oregon, Ctr High Energy Phys, Eugene, OR USA.
[Abeloos, B.; Ayoub, M. K.; Bassalat, A.; Binet, S.; Bourdarios, C.; De Regie, J. B. De Vivie; Delgove, D.; Duflot, L.; Escalier, M.; Fayard, L.; Fournier, D.; Gkougkousis, E. L.; Goudet, C. R.; Grivaz, J. -F.; Hariri, F.; Henrot-Versille, S.; Hrivnac, J.; Iconomidou-Fayard, L.; Kado, M.; Lounis, A.; Maiani, C.; Makovec, N.; Morange, N.; Nellist, C.; Petroff, P.; Poggioli, L.; Puzo, P.; Rousseau, D.; Rybkin, G.; Schaffer, A. C.; Serin, L.; Simion, S.; Tanaka, R.; Zerwas, D.; Zhang, Z.] Univ Paris 11, LAL, CNRS, IN2P3, Orsay, France.
[Ishijima, N.; Nomachi, M.; Sugaya, Y.; Teoh, J. J.; Yamaguchi, Y.] Osaka Univ, Grad Sch Sci, Osaka, Japan.
[Bugge, M. K.; Cameron, D.; Catmore, J. R.; Feigl, S.; Franconi, L.; Garonne, V.; Gjelsten, B. K.; Gramstad, E.; Morisbak, V.; Nilsen, J. K.; Ould-Saada, F.; Pajchel, K.; Pedersen, M.; Raddum, S.; Read, A. L.; Rohne, O.; Sandaker, H.; Serfon, C.; Stapnes, S.; Strandlie, A.] Univ Oslo, Dept Phys, Oslo, Norway.
[Artoni, G.; Backes, M.; Barr, A. J.; Becker, K.; Beresford, L.; Bortoletto, D.; Burr, J. T. P.; Cooper-Sarkar, A. M.; Ortuzar, M. Crispin; Fawcett, W. J.; Frost, J. A.; Gallas, E. J.; Giuli, F.; Gupta, S.; Gwenlan, C.; Hays, C. P.; Henderson, J.; Huffman, T. B.; Issever, C.; Kalderon, C. W.; Nagai, K.; Nickerson, R. B.; Norjoharuddeen, N.; Petrov, M.; Pickering, M. A.; Radescu, V.; Tseng, J. C-L.; Viehhauser, G. H. A.; Vigani, L.; Weidberg, A. R.; Zhong, J.] Univ Oxford, Dept Phys, Oxford, England.
[Ferrari, R.; Gaudio, G.; Lanza, A.; Polesello, G.; Vercesi, V.] INFN Sezione Pavia, Pavia, Italy.
[Dondero, P.; Farina, E. M.; Fraternali, M.; Introzzi, G.; Kourkoumeli-Charalampidi, A.; Livan, M.; Negri, A.; Rebuzzi, D. M.; Rimoldi, A.] Univ Pavia, Dipartimento Fis, Pavia, Italy.
[Balunas, W. K.; Brendlinger, K.; Di Clemente, W. K.; Fletcher, R. R. M.; Haney, B.; Heim, S.; Hines, E.; Jackson, B.; Kroll, J.; Lipeles, E.; Meyer, C.; Mistry, K. P.; Reichert, J.; Schaefer, L.; Thomson, E.; Vanguri, R.; Williams, H. H.; Yoshihara, K.] Univ Penn, Dept Phys, Philadelphia, PA 19104 USA.
[Basalaev, A.; Ezhilov, A.; Fedin, O. L.; Gratchev, V.; Levchenko, M.; Maleev, V. P.; Naryshkin, I.; Ryabov, Y. F.; Schegelsky, V. A.; Seliverstov, D. M.; Solovyev, V.] Natl Res Ctr Kurchatov, Inst BP Konstantinov Peter, St Petersburg, Russia.
INFN, Sez Pisa, Pisa, Italy.
[Annovi, A.; Bertolucci, F.; Biesuz, N. V.; Cavasinni, V.; Chiarelli, G.; Del Prete, T.; Dell'Orso, M.; Donati, S.; Giannetti, P.; Leone, S.; Roda, C.; Scuri, F.; Sotiropoulou, C. L.; Spalla, M.; Volpi, G.] Univ Pisa, Dipartimento Fis Fermi, Pisa, Italy.
[Bianchi, R. M.; Boudreau, J.; Escobar, C.; Farina, C.; Hong, T. M.; Mueller, J.; Sapp, K.; Su, J.] Univ Pittsburgh, Dept Phys & Astron, Pittsburgh, PA 15260 USA.
[Araque, J. P.; Castro, N. F.; Seabra, L. F. Oleiro; Santos, H.] Lab Instrumental Fis Expt Particulas LIP, Lisbon, Portugal.
[Amorim, A.; Muio, P. Conde; Da Cunha Sargedas De Sousa, M. J.; Jorge, P. M.; Miguens, J. Machado; Maneira, J.; Pedro, R.; Delgado, A. Tavares] Univ Lisbon, Fac Cincias, Lisbon, Portugal.
[Dos Santos, S. P. Amor; Carvalho, J.; Fiolhais, M. C. N.; Galhardo, B.; Veloso, F.; Wolters, H.] Univ Coimbra, Dept Phys, Coimbra, Portugal.
[Gomes, A.; Maio, A.; Saraiva, J. G.; Silva, J.] Univ Lisbon, Ctr Fis Nucl, Lisbon, Portugal.
[Onofre, A.] Univ Minho, Dept Fis, Braga, Portugal.
[Aguilar-Saavedra, J. A.] Univ Granada, Dept Fis Teor Cosmos, CAFPE, Granada, Spain.
Univ Nova Lisboa, Dep Fis & CEFITEC, Fac Ciencias Tecnol, Caparica, Portugal.
[Chudoba, J.; Havranek, M.; Hejbal, J.; Jakoubek, T.; Kepka, O.; Kupco, A.; Kus, V.; Lokajicek, M.; Lysak, R.; Marcisovsky, M.; Mikestikova, M.; Nemecek, S.; Penc, O.; Sicho, P.; Staroba, P.; Svatos, M.; Tasevsky, M.; Vrba, V.] Acad Sci Czech Republic, Inst Phys, Prague, Czech Republic.
[Ali, B.; Augsten, K.; Caforio, D.; Gallus, P.; Hubacek, Z.; Myska, M.; Pospisil, S.; Seifert, F.; Simak, V.; Slavicek, T.; Smolek, K.; Solar, M.; Sopczak, A.; Sopko, V.; Suk, M.; Turecek, D.; Vacek, V.; Vlasak, M.; Vokac, P.; Vykydal, Z.; Zeman, M.] Czech Tech Univ, Prague, Czech Republic.
[Berta, P.; Carli, I.; Davidek, T.; Dolejsi, J.; Dolezal, Z.; Kodys, P.; Kosek, T.; Leitner, R.; Mlynarikova, M.; Reznicek, P.; Scheirich, D.; Slovak, R.; Spousta, M.; Sykora, T.; Tas, P.; Todorova-Nova, S.; Valkar, S.; Vorobel, V.] Charles Univ Prague, Fac Math & Phys, Prague, Czech Republic.
[Borisov, A.; Cheremushkina, E.; Denisov, S. P.; Fakhrutdinov, R. M.; Fenyuk, A. B.; Golubkov, D.; Kamenshchikov, A.; Karyukhin, A. N.; Kozhin, A. S.; Minaenko, A. A.; Myagkov, A. G.; Nikolaenko, V.; Ryzhov, A.; Solodkov, A. A.; Solovyanov, O. V.; Starchenko, E. A.; Zaitsev, A. M.; Zenin, O.] State Res Ctr Inst High Energy Phys Protvino, NRC KI, Protvino, Russia.
[Adye, T.; Baines, J. T.; Barnett, B. M.; Burke, S.; Dewhurst, A.; Dopke, J.; Emeliyanov, D.; Gallop, B. J.; Gee, C. N. P.; Haywood, S. J.; Kirk, J.; Martin-Haugh, S.; McMahon, S. J.; Middleton, R. P.; Phillips, P. W.; Sankey, D. P. C.; Sawyer, C.; Tyndel, M.; Wickens, F. J.; Wielers, M.; Worm, S. D.] Rutherford Appleton Lab, Particle Phys Dept, Didcot, Oxon, England.
[Acharya, B. S.; Anulli, F.; De Pedis, D.; De Salvo, A.; Falciano, S.; Luminari, L.; Nisati, A.; Pasqualucci, E.; Petrolo, E.; Pinamonti, M.; Pontecorvo, L.; Rescigno, M.; Rosati, S.; Tehrani, F. Safai; Vari, R.; Veneziano, S.] INFN, Sez Roma, Rome, Italy.
[Bagiacchi, P.; Bagnaia, P.; Bauce, M.; Bini, C.; Ciapetti, G.; Corradi, M.; Di Donato, C.; Gentile, S.; Giagu, S.; Gustavino, G.; Kuna, M.; Lacava, F.; Luci, C.; Messina, A.; Vanadia, M.; Verducci, M.; Zanello, L.] Sapienza Univ Roma, Dipartimento Fis, Rome, Italy.
[Cardarelli, R.; Liberti, B.] INFN, Sez Roma Tor Vergata, Rome, Italy.
[Aielli, G.; Camarri, P.; Cerrito, L.; Di Ciaccio, A.; Salamon, A.; Santonico, R.] Univ Roma Tor Vergata, Dipartimento Fis, Rome, Italy.
[Baroncelli, A.; Biglietti, M.; Farilla, A.; Graziani, E.; Iodice, M.; Stanescu, C.] INFN, Sez Roma Tre, Rome, Italy.
[Ceradini, F.; Di Micco, B.; Orestano, D.; Petrucci, F.; Puddu, D.; Salamanna, G.; Sessa, M.; Taccini, C.] Univ Roma Tre, Dipartimento Matemat Fis, Rome, Italy.
[Benchekroun, D.; Chafaq, A.; Hoummada, A.] Seau Univ Phys Hautes Energies Univ, Fac Sci Ain Chock Hassan II, Casablanca, Morocco.
Ctr Natl Energie Sci Tech Nucl, Rabat, Morocco.
[El Kacimi, M.; Goujdami, D.] LPHEA Marrakech Univ, Fac Sci Semlalia, Marrakech, Morocco.
[Aaboud, M.; Derkaoui, J. E.; Ouchrif, M.] Univ Mohamed Premier, Fac Sci, LPTPM, Oujda, Morocco.
[El Moursli, R. Cherkaoui; Ezzi, M.; Fassi, F.; Haddad, N.; Idrissi, Z.; Tayalati, Y.] Univ Mohammaed, Fac Sci, Rabat, Morocco.
[Bachacou, H.; Balli, F.; Bauer, F.; Besson, N.; Blanchard, J. -B.; Boonekamp, M.; Chevalier, L.; Hoffmann, M. Dano; Deliot, F.; Denysiuk, D.; Etienvre, A. I.; Formica, A.; Giraud, P. F.; Da Costa, J. Goncalves Pinto Firmino; Guyot, C.; Hanna, R.; Hassani, S.; Jeanneau, F.; Kivernyk, O.; Kozanecki, W.; Kukla, R.; Laporte, J. F.; Le Quilleuc, E. P.; Lesage, A. A. J.; Mansoulie, B.; Meyer, J-P.; Nicolaidou, R.; Ouraou, A.; Rodriguez, L. Pacheco; Perego, M. M.; Peyaud, A.; Saimpert, M.; Schoeffel, L.; Schune, Ph.; Schwemling, Ph.; Schwindling, J.] CEA Saclay, DSM IRFU Inst Rech Lois Fondament Universe, Gif Sur Yvette, France.
[AbouZeid, O. S.; Battaglia, M.; Debenedetti, C.; Grillo, A. A.; Hance, M.; Kuhl, A.; Law, A. T.; Litke, A. M.; Lockman, W. S.; Nielsen, J.; Reece, R.; Rose, P.; Sadrozinski, H. F-W.; Schier, S.; Schumm, B. A.; Seiden, A.] Univ Calif Santa Cruz, Santa Cruz Inst Particle Phys, Santa Cruz, CA 95064 USA.
[Alpigiani, C.; Blackburn, D.; Goussiou, A. G.; Hsu, S. -C.; Johnson, W. J.; Lubatti, H. J.; Marx, M.; Meehan, S.; Rompotis, N.; Rosten, R.; Rothberg, J.; Russell, H. L.; De Bruin, P. H. Sales; Pastor, E. Torr; Watts, G.; Whallon, N. L.] Univ Washington, Dept Phys, Seattle, WA USA.
[Du, Y.; Feng, C.; Ma, L. L.; Ma, Y.; Wang, C.; Zhang, X.; Zhao, Y.; Zhu, C. G.] Shandong Univ, Sch Phys, Shandong, Peoples R China.
[Bret, M. Cano; Guo, J.; Hu, S.; Li, L.; Yang, H.] Shanghai Jiao Tong Univ, Dept Phys & Astron, Shanghai Key Lab Particle Phys & Cosmol, Shanghai, Peoples R China.
[Anastopoulos, C.; Costanzo, D.; Donszelmann, T. Cuhadar; Dawson, I.; Fletcher, G. T.; Hamity, G. N.; Hodgkinson, M. C.; Hodgson, P.; Johansson, P.; Klinger, J. A.; Korolkova, E. V.; Kyriazopoulos, D.; Paredes, B. Lopez; Macdonald, C. M.; Miyagawa, P. S.; Parker, K. A.; Tovey, D. R.; Vickey, T.; Boeriu, O. E. Vickey] Univ Sheffield, Dept Phys & Astron, Sheffield, S Yorkshire, England.
[Hasegawa, Y.; Takeshita, T.] Shinshu Univ, Dept Phys, Nagano, Japan.
[Atlay, N. B.; Buchholz, P.; Campoverde, A.; Czirr, H.; Fleck, I.; Ghasemi, S.; Ibragimov, I.; Li, Y.; Walkowiak, W.; Ziolkowski, M.] Univ Siegen, Fachbereich Phys, Siegen, Germany.
[Buat, Q.; Horton, A. J.; Mori, D.; O'Neil, D. C.; Pachal, K.; Stelzer, B.; Temple, D.; Torres, H.; Van Nieuwkoop, J.; Vetterli, M. C.] Simon Fraser Univ, Dept Phys, Burnaby, BC, Canada.
[Armbruster, A. J.; Barklow, T.; Bartoldus, R.; Bawa, H. S.; Black, J. E.; Gao, Y. S.; Garelli, N.; Grenier, P.; Ilic, N.; Kagan, M.; Kocian, M.; Koi, T.; Malone, C.; Moss, J.; Mount, R.; Nachman, B. P.; Piacquadio, G.; Rubbo, F.; Salnikov, A.; Schwartzman, A.; Su, D.; Tompkins, L.; Wittgen, M.; Young, C.; Zeng, Q.] SLAC Natl Accelerator Lab, Stanford, CA USA.
[Astalos, R.; Bartos, P.; Blazek, T.; Dado, T.; Melo, M.; Plazak, L.; Smiesko, J.; Sykora, I.; Tokar, S.; Zenis, T.] Comenius Univ, Fac Math Phys & Informat, Bratislava, Slovakia.
[Bruncko, D.; Kladiva, E.; Strizenec, P.; Urban, J.] Slovak Acad Sci, Inst Expt Phys, Dept Subnucl Phys, Kosice, Slovakia.
[Castaneda-Miranda, E.; Hamilton, A.; Yacoob, S.] Univ Cape Town, Dept Phys, Cape Town, South Africa.
[Connell, S. H.; Govender, N.] Univ Johannesburg, Dept Phys, Johannesburg, South Africa.
[Hsu, C.; Jivan, H.; Kar, D.; Garcia, B. R. Mellado; Reed, R. G.; Ruan, X.] Univ Witwatersrand, Sch Phys, Johannesburg, South Africa.
[Bohm, C.; Silverstein, S. B.] Stockholm Univ, Dept Phys, Stockholm, Sweden.
[Abulaiti, Y.; Akerstedt, H.; Asman, B.; Bendtz, K.; Bertoli, G.; Bylund, O. Bessidskaia; Clement, C.; Cribbs, W. A.; Gellerstedt, K.; Hellman, S.; Jon-And, K.; Lundberg, O.; Milstead, D. A.; Moa, T.; Molander, S.; Pani, P.; Poettgen, R.; Rossetti, V.; Shaikh, N. W.; Shcherbakova, A.; Sjolin, J.; Strandberg, S.; Ughetto, M.; Santurio, E. Valdes; Wallangen, V.] Oskar Klein Ctr, Stockholm, Sweden.
[Lund-Jensen, B.; Sidebo, P. E.; Strandberg, J.] Royal Inst Technol, Dept Phys, Stockholm, Sweden.
[Balestri, T.; Bee, C. P.; Chen, K.; Hobbs, J.; Huo, P.; Jia, J.; Li, H.; Lindquist, B. E.; McCarthy, R. L.; Montalbano, A.; Morvaj, L.; Radhakrishnan, S. K.; Rijssenbeek, M.; Schamberger, R. D.; Tsybychev, D.; Zaman, A.; Zhou, M.] SUNY Stony Brook, Dept Phys & Astron & Chem, Stony Brook, NY 11794 USA.
[Abraham, N. L.; Allbrooke, B. M. M.; Asquith, L.; Cerri, A.; Barajas, C. A. Chavez; De Sanctis, U.; De Santo, A.; Lerner, G.; Miano, F.; Salvatore, F.; Castillo, I. Santoyo; Shehu, C. Y.; Suruliz, K.; Sutton, M. R.; Vivarelli, I.; Winston, O. J.] Univ Sussex, Dept Phys & Astron, Brighton, E Sussex, England.
[Black, C. W.; Finelli, K. D.; Jeng, G. -Y.; Limosani, A.; Morley, A. K.; Saavedra, A. F.; Scarcella, M.; Varvell, K. E.; Wang, J.; Yabsley, B.] Univ Sydney, Sch Phys, Sydney, NSW, Australia.
[Hou, S.; Hsu, P. J.; Lee, S. C.; Lin, S. C.; Liu, B.; Liu, D.; Lo Sterzo, F.; Mazini, R.; Shi, L.; Soh, D. A.; Teng, P. K.; Wang, S. M.; Yang, Y.] Acad Sinica, Inst Phys, Taipei, Taiwan.
[Abreu, H.; Gozani, E.; Rozen, Y.; Tarem, S.; van Eldik, N.] Technion Israel Inst Technol, Dept Phys, Haifa, Israel.
[Abramowicz, H.; Alexander, G.; Ashkenazi, A.; Bella, G.; Benary, O.; Benhammou, Y.; Davies, M.; Duarte-Campderros, J.; Etzion, E.; Gershon, A.; Gueta, O.; Oren, Y.; Soffer, A.; Taiblum, N.] Tel Aviv Univ, Raymond & Beverly Sackler Sch Phys & Astron, Tel Aviv, Israel.
[Gentsos, C.; Gkaitatzis, S.; Gkialas, I.; Iliadis, D.; Kimura, N.; Kordas, K.; Papageorgiou, K.; Petridou, C.; Sampsonidis, D.] Aristotle Univ Thessaloniki, Dept Phys, Thessaloniki, Greece.
[Adachi, S.; Asai, S.; Chen, S.; Enari, Y.; Hanawa, K.; Ishino, M.; Kanaya, N.; Kataoka, Y.; Kato, C.; Kawamoto, T.; Kishimoto, T.; Kobayashi, A.; Kobayashi, T.; Komori, Y.; Kozakai, C.; Mashimo, T.; Masubuchi, T.; Minami, Y.; Minegishi, Y.; Mori, T.; Morinaga, M.; Nakamura, T.; Ninomiya, Y.; Nobe, T.; Okumura, Y.; Saito, T.; Sakamoto, H.; Tanaka, J.; Terashi, K.; Ueda, I.; Yamamoto, S.; Yamanaka, T.] Univ Tokyo, Int Ctr Elementary Particle Phys, Dept Phys, Tokyo, Japan.
[Bratzler, U.; Fukunaga, C.] Tokyo Metropolitan Univ, Grad Sch Sci & Technol, Tokyo, Japan.
[Hayakawa, D.; Ishitsuka, M.; Jinnouchi, O.; Kobayashi, D.; Kuze, M.; Motohashi, K.; Tanaka, M.; Todome, K.; Yamaguchi, D.] Tokyo Inst Technol, Dept Phys, Tokyo, Japan.
[Vaniachine, A.] Tomsk State Univ, Tomsk, Russia.
[Batista, S. J.; Chau, C. C.; Cormier, K. J. R.; DeMarco, D. A.; Di Sipio, R.; Diamond, M.; Keoshkerian, H.; Krieger, P.; Liblong, A.; Mc Goldrick, G.; Orr, R. S.; Pascuzzi, V. R.; Polifka, R.; Rudolph, M. S.; Savard, P.; Sinervo, P.; Taenzer, J.; Teuscher, R. J.; Trischuk, W.; Veloce, L. M.; Venturi, N.] Univ Toronto, Dept Phys, Toronto, ON, Canada.
INFN TIFPA, Povo, Italy.
[Iuppa, R.] Univ Trento, Trento, Italy.
[Canepa, A.; Chekulaev, S. V.; Hod, N.; Jovicevic, J.; Codina, E. Perez; Schneider, B.; Stelzer-Chilton, O.; Tafirout, R.; Trigger, I. M.] TRIUMF, Vancouver, BC, Canada.
[Ramos, J. Manjarres; Palacino, G.; Taylor, W.] York Univ, Dept Phys & Astron, Toronto, ON, Canada.
[Hagihara, M.; Hara, K.; Ito, F.; Kasahara, K.; Kim, S. H.; Kiuchi, K.; Nagata, K.; Okawa, H.; Sato, K.; Ukegawa, F.] Univ Tsukuba, Fac Pure & Appl Sci, Ctr Integrated Res Fundamental Sci & Engn, Tsukuba, Ibaraki, Japan.
[Beauchemin, P. H.; Meoni, E.; Sliwa, K.; Son, H.; Wetter, J.] Tufts Univ, Dept Phys & Astron, Medford, MA 02155 USA.
[Casper, D. W.; Colombo, T.; Corso-Radu, A.; Frate, M.; Guest, D.; Lankford, A. J.; Mete, A. S.; Nelson, A.; Ntekas, K.; Scannicchio, D. A.; Schernau, M.; Shimmin, C. O.; Taffard, A.; Unel, G.; Whiteson, D.] Univ Calif Irvine, Dept Phys & Astron, Irvine, CA USA.
INFN, Sez Trieste, Grp Coll Udine, Udine, Italy.
[Quayle, W. B.; Serkin, L.; Shaw, K.] Abdus Salaam Int Ctr Theoret Phys, Trieste, Italy.
[Boldyrev, A. S.; Cheatham, S.; Cobal, M.; Giordani, M. P.; Soualah, R.; Truong, L.] Univ Udine, Dipartimento Chim Fis Ambiente, Udine, Italy.
[Kuutmann, E. Bergeaas; Brenner, R.; Ekelof, T.; Ellert, M.; Ferrari, A.; Maddocks, H. J.; Ohman, H.; Rangel-Smith, C.] Uppsala Univ, Dept Phys & Astron, Uppsala, Sweden.
[Atkinson, M.; Armadans, R. Caminal; Cavaliere, V.; Chang, P.; Errede, S.; Hooberman, B. H.; Khader, M.; Lie, K.; Liss, T. M.; Liu, L.; Long, J. D.; Outschoorn, V. I. Martinez; Neubauer, M. S.; Rybar, M.; Shang, R.; Sickles, A. M.; Vichou, I.; Zeng, J. C.] Univ Illinois, Dept Phys, 1110 W Green St, Urbana, IL 61801 USA.
[Piqueras, D. Alvarez; Navarro, L. Barranco; Urban, S. Cabrera; Gimenez, V. Castillo; Alberich, L. Cerda; Costa, M. J.; Martinez, P. Fernandez; Ferrer, A.; Fiorini, L.; Fuster, J.; Garcia, C.; Navarro, J. E. Garcia; Gonzalez de la Hoz, S.; Hernandez Jimenez, Y.; Hign-Rodriguez, E.; Pena, J. Jimenez; King, M.; Lacasta, C.; Lacuesta, V. R.; Mamuzic, J.; Marti-Garcia, S.; Melini, D.; Mitsou, V. A.; Lopez, S. Pedraza; Rodriguez, D.; Adam, E. Romero; Ros, E.; Salt, J.; Sanchez, J.; Martinez, V. Sanchez; Soldevila, U.; Valero, A.; Ferrer, J. A. Valls; Vos, M.] Univ Valencia, Inst Fis Corpuscular IFIC, Dept Ingn Elect, CSIC,Dept Fis & Astron,Inst Microelect, Valencia, Spain.
[Danninger, M.; Fedorko, W.; Gay, C.; Gecse, Z.; Gignac, M.; Henkelmann, S.; Lister, A.] Univ British Columbia, Dept Phys, Vancouver, BC, Canada.
[Albert, J.; David, C.; Elliot, A. A.; Fincke-Keeler, M.; Hamano, K.; Hill, E.; Keeler, R.; Kowalewski, R.; Kuwertz, E. S.; Kwan, T.; LeBlanc, M.; Lefebvre, M.; McPherson, R. A.; Pearce, J.; Seuster, R.; Sobie, R.; Trovatelli, M.; Venturi, M.] Univ Victoria, Dept Phys & Astron, Victoria, BC, Canada.
[Beckingham, M.; Ennis, J. S.; Farrington, S. M.; Harrison, P. F.; Jeske, C.; Jones, G.; Martin, T. A.; Murray, W. J.; Pianori, E.; Spangenberg, M.] Univ Warwick, Dept Phys, Coventry, W Midlands, England.
[Iizawa, T.; Kaji, T.; Mitani, T.; Sakurai, Y.; Yorita, K.] Waseda Univ, Tokyo, Japan.
[Balek, P.; Bressler, S.; Citron, Z. H.; Duchovni, E.; Dumancic, M.; Gross, E.; Kohler, M. K.; Lellouch, D.; Levinson, L. J.; Mikenberg, G.; Milov, A.; Pitt, M.; Ravinovich, I.; Roth, I.; Schaarschmidt, J.; Smakhtin, V.; Turgeman, D.] Weizmann Inst Sci, Dept Particle Phys, Rehovot, Israel.
[Banerjee, Sw.; Guan, W.; Hard, A. S.; Heng, Y.; Ji, H.; Ju, X.; Kaplan, L. S.; Kashif, L.; Ming, Y.; Wang, F.; Wiedenmann, W.; Wu, S. L.; Yang, H.; Zhang, F.; Zhou, C.; Zobernig, G.] Univ Wisconsin, Dept Phys, Madison, WI USA.
[Herget, V.; Kuger, F.; Redelbach, A.; Schreyer, M.; Sidiropoulou, O.; Siragusa, G.; Strohmer, R.; Trefzger, T.; Weber, S. W.; Zibell, A.] Univ Wurzburg, Fak Phys & Astron, Wurzburg, Germany.
[Bannoura, A. A. E.; Boerner, D.; Cornelissen, T.; Ellinghaus, F.; Ernis, G.; Fischer, J.; Flick, T.; Gabizon, O.; Gilles, G.; Hamacher, K.; Harenberg, T.; Hirschbuehl, D.; Kersten, S.; Kuechler, J. T.; Mattig, P.; Neumann, M.; Pataraia, S.; Riegel, C. J.; Sandhoff, M.; Tepel, F.; Vogel, M.; Wagner, W.; Zeitnitz, C.] Berg Univ Wuppertal, Fak Math & Nat Wissensch, Fachgrp Phys, Wuppertal, Germany.
[Baker, O. K.; Noccioli, E. Benhar; Cummings, J.; Demers, S.; Ideal, E.; Lagouri, T.; Leister, A. G.; Loginov, A.; Paganini, M.; Hernandez, D. Paredes; Thomsen, L. A.; Tipton, P.; Vasquez, J. G.; Wang, X.] Yale Univ, Dept Phys, New Haven, CT USA.
[Hakobyan, H.; Vardanyan, G.] Yerevan Phys Inst, Yerevan, Armenia.
[Rahal, G.] Ctr Calcul, IN2P3, Villeurbanne, France.
[ATLAS Collaboration] CERN, CH-1211 Geneva 23, Switzerland.
RP Aaboud, M (reprint author), Seau Univ Phys Hautes Energies Univ, Fac Sci Ain Chock Hassan II, Casablanca, Morocco.
RI Mitsou, Vasiliki/D-1967-2009; Tikhomirov, Vladimir/M-6194-2015; Owen,
Mark/Q-8268-2016; Gladilin, Leonid/B-5226-2011; Livan,
Michele/D-7531-2012; Doyle, Anthony/C-5889-2009; Boyko,
Igor/J-3659-2013; Shulga, Evgeny/R-1759-2016; Carvalho,
Joao/M-4060-2013; Lazzaroni, Massimo/N-3675-2015; Maleev,
Victor/R-4140-2016; Warburton, Andreas/N-8028-2013; Snesarev,
Andrey/H-5090-2013; Solodkov, Alexander/B-8623-2017; Zaitsev,
Alexandre/B-8989-2017; Leitner, Rupert/C-2004-2017; Carli,
Ina/C-2189-2017; messina, andrea/C-2753-2013; Guo, Jun/O-5202-2015;
Villa, Mauro/C-9883-2009; Peleganchuk, Sergey/J-6722-2014; Yang,
Haijun/O-1055-2015; Li, Liang/O-1107-2015; Monzani, Simone/D-6328-2017;
Kuday, Sinan/C-8528-2014; della Volpe, Domenico/B-4482-2012; Brooks,
William/C-8636-2013; Camarri, Paolo/M-7979-2015; Prokoshin,
Fedor/E-2795-2012; Mindur, Bartosz/A-2253-2017; Ventura,
Andrea/A-9544-2015; Mashinistov, Ruslan/M-8356-2015; Gutierrez,
Phillip/C-1161-2011; Fabbri, Laura/H-3442-2012; White, Ryan/E-2979-2015;
Kantserov, Vadim/M-9761-2015; Chekulaev, Sergey/O-1145-2015; Zhukov,
Konstantin/M-6027-2015
OI Mitsou, Vasiliki/0000-0002-1533-8886; Tikhomirov,
Vladimir/0000-0002-9634-0581; Owen, Mark/0000-0001-6820-0488; Gladilin,
Leonid/0000-0001-9422-8636; Livan, Michele/0000-0002-5877-0062; Doyle,
Anthony/0000-0001-6322-6195; Boyko, Igor/0000-0002-3355-4662; Shulga,
Evgeny/0000-0001-5099-7644; Carvalho, Joao/0000-0002-3015-7821;
Lazzaroni, Massimo/0000-0002-4094-1273; Warburton,
Andreas/0000-0002-2298-7315; Solodkov, Alexander/0000-0002-2737-8674;
Zaitsev, Alexandre/0000-0002-4961-8368; Leitner,
Rupert/0000-0002-2994-2187; Carli, Ina/0000-0002-0411-1141; Guo,
Jun/0000-0001-8125-9433; Villa, Mauro/0000-0002-9181-8048; Peleganchuk,
Sergey/0000-0003-0907-7592; Li, Liang/0000-0001-6411-6107; Monzani,
Simone/0000-0002-0479-2207; Kuday, Sinan/0000-0002-0116-5494; Brooks,
William/0000-0001-6161-3570; Camarri, Paolo/0000-0002-5732-5645;
Prokoshin, Fedor/0000-0001-6389-5399; Mindur,
Bartosz/0000-0002-5511-2611; Ventura, Andrea/0000-0002-3368-3413;
Mashinistov, Ruslan/0000-0001-7925-4676; Fabbri,
Laura/0000-0002-4002-8353; White, Ryan/0000-0003-3589-5900; Kantserov,
Vadim/0000-0001-8255-416X;
FU ANPCyT, Argentina; YerPhI, Armenia; ARC, Australia; BMWFW, Austria; FWF,
Austria; ANAS, Azerbaijan; SSTC, Belarus; CNPq, Brazil; FAPESP, Brazil;
NSERC, Canada; NRC, Canada; CFI, Canada; CERN; CONICYT, Chile; CAS,
China; MOST, China; NSFC, China; COLCIENCIAS, Colombia; MSMT CR, Czech
Republic; MPO CR, Czech Republic; VSC CR, Czech Republic; DNRF, Denmark;
DNSRC, Denmark; IN2P3-CNRS, France; CEA-DSM/IRFU, France; GNSF, Georgia;
BMBF, Germany; HGF, Germany; MPG, Germany; GSRT, Greece; RGC, China;
Hong Kong SAR, China; ISF, Israel; I-CORE, Israel; Benoziyo Center,
Israel; INFN, Italy; MEXT, Japan; JSPS, Japan; CNRST, Morocco; FOM,
Netherlands; NWO, Netherlands; RCN, Norway; MNiSW, Poland; NCN, Poland;
FCT, Portugal; MNE/IFA, Romania; MES of Russia, Russian Federation; NRC
KI, Russian Federation; JINR; MESTD, Serbia; MSSR, Slovakia; ARRS,
Slovenia; MIZS, Slovenia; DST/NRF, South Africa; MINECO, Spain; SRC,
Sweden; Wallenberg Foundation, Sweden; SERI, Switzerland; SNSF,
Switzerland; Cantons of Bern and Geneva, Switzerland; MOST, Taiwan;
TAEK, Turkey; STFC, United Kingdom; DOE, USA; NSF, USA; BCKDF, Canada;
Canada Council, Canada; CANARIE, Canada; CRC, Canada; Compute Canada,
Canada; FQRNT, Canada; Ontario Innovation Trust, Canada; EPLANET,; ERC;
FP7, Horizon 2020 and Marie Sklodowska-Curie Actions; European Union;
Investissements d'Avenir Labex and Idex, France; ANR, France; Region
Auvergne and Fondation Partager le Savoir, France; DFG, Germany; AvH
Foundation, Germany; Herakleitos, Thales and Aristeia programmes by
EU-ESF; Greek NSRF; BSF, Israel; GIF, Israel; Minerva, Israel; BRF,
Norway; Generalitat de Catalunya, Spain; Generalitat Valenciana, Spain;
Royal Society and Leverhulme Trust, UK
FX We thank CERN for the very successful operation of the LHC, as well as
the support staff from our institutions without whom ATLAS could not be
operated efficiently. We acknowledge the support of ANPCyT, Argentina;
YerPhI, Armenia; ARC, Australia; BMWFW and FWF, Austria; ANAS,
Azerbaijan; SSTC, Belarus; CNPq and FAPESP, Brazil; NSERC, NRC and CFI,
Canada; CERN; CONICYT, Chile; CAS, MOST and NSFC, China; COLCIENCIAS,
Colombia; MSMT CR, MPO CR and VSC CR, Czech Republic; DNRF and DNSRC,
Denmark; IN2P3-CNRS, CEA-DSM/IRFU, France; GNSF, Georgia; BMBF, HGF, and
MPG, Germany; GSRT, Greece; RGC, Hong Kong SAR, China; ISF, I-CORE and
Benoziyo Center, Israel; INFN, Italy; MEXT and JSPS, Japan; CNRST,
Morocco; FOM and NWO, Netherlands; RCN, Norway; MNiSW and NCN, Poland;
FCT, Portugal; MNE/IFA, Romania; MES of Russia and NRC KI, Russian
Federation; JINR; MESTD, Serbia; MSSR, Slovakia; ARRS and MIZS,
Slovenia; DST/NRF, South Africa; MINECO, Spain; SRC and Wallenberg
Foundation, Sweden; SERI, SNSF and Cantons of Bern and Geneva,
Switzerland; MOST, Taiwan; TAEK, Turkey; STFC, United Kingdom; DOE and
NSF, USA. In addition, individual groups and members have received
support from BCKDF, the Canada Council, CANARIE, CRC, Compute Canada,
FQRNT, and the Ontario Innovation Trust, Canada; EPLANET, ERC, FP7,
Horizon 2020 and Marie Sklodowska-Curie Actions, European Union;
Investissements d'Avenir Labex and Idex, ANR, Region Auvergne and
Fondation Partager le Savoir, France; DFG and AvH Foundation, Germany;
Herakleitos, Thales and Aristeia programmes co-financed by EU-ESF and
the Greek NSRF; BSF, GIF and Minerva, Israel; BRF, Norway; Generalitat
de Catalunya, Generalitat Valenciana, Spain; the Royal Society and
Leverhulme Trust, UK. The crucial computing support from all WLCG
partners is acknowledged gratefully, in particular from CERN, the ATLAS
Tier-1 facilities at TRIUMF (Canada), NDGF (Denmark, Norway, Sweden),
CC-IN2P3 (France), KIT/GridKA (Germany), INFN-CNAF (Italy), NLT1
(Netherlands), PIC (Spain), ASGC (Taiwan), RAL (UK) and BNL (USA), the
Tier-2 facilities worldwide and large non-WLCG resource providers. Major
contributors of computing resources are listed in Ref. [77].
NR 77
TC 0
Z9 0
U1 67
U2 67
PU SPRINGER
PI NEW YORK
PA 233 SPRING ST, NEW YORK, NY 10013 USA
SN 1434-6044
EI 1434-6052
J9 EUR PHYS J C
JI Eur. Phys. J. C
PD OCT 4
PY 2016
VL 76
IS 10
AR 541
DI 10.1140/epjc/s10052-016-4385-1
PG 28
WC Physics, Particles & Fields
SC Physics
GA DY5ZT
UT WOS:000385185400001
PM 28316486
ER
PT J
AU Poirier, I
Kuhn, L
Demortiere, A
Mirvaux, B
Hammann, P
Chicher, J
Caplat, C
Pallud, M
Bertrand, M
AF Poirier, Isabelle
Kuhn, Lauriane
Demortiere, Arnaud
Mirvaux, Boris
Hammann, Philippe
Chicher, Johana
Caplat, Christelle
Pallud, Marie
Bertrand, Martine
TI Ability of the marine bacterium Pseudomonas fluorescens BA3SM1 to
counteract the toxicity of CdSe nanoparticles
SO JOURNAL OF PROTEOMICS
LA English
DT Article
DE Marine bacteria; CdSe nanoparticles; Physiological responses;
Proteomics; Oxidative stress
ID SEMICONDUCTOR QUANTUM DOTS; ESCHERICHIA-COLI; SILVER NANOPARTICLES;
OXIDATIVE STRESS; BIOFILM FORMATION; OXIDE NANOPARTICLES; CHLORORAPHIS
O6; METAL-IONS; CADMIUM; AERUGINOSA
AB In the marine environment, bacteria from estuarine and coastal sediments are among the first targets of nanopartide pollution; it is therefore relevant to improve the knowledge of interactions between bacteria and nanoparticles. In this work, the response of the marine bacterium Pseudomonas fluorescens BA3SM1 to CdSe nanocrystals (CdSe NPs) of 3 nm (NP3) and 8 nm (NP8) in diameter was evaluated through microscopic, physiological, biochemical and proteomic approaches. Transmission electron microscopy images showed that NP3 were able to penetrate the bacteria, while NP8 were highly concentrated around the cells, embedded in large exopolysaccharides. In our experimental conditions, both CdSe NP sizes induced a decrease in respiration during the stationary growth phase, while only NP8 caused growth retardation and a decrease in pyoverdine production. Proteomic analyses highlighted that the strain responded to CdSe NP toxicity by inducing various defence mechanisms such as cell aggregation, extracellular CdSe NP sequestration, effective protection against oxidative stress, modifications of envelope organization and properties, and cadmium export. In addition, BA3SM1 presented a biosorption capacity of 1.6 x 10(16) NP3/g dry weight and 1.7 x 10(15) NP8/g dry weight. This strain therefore appears as a promising agent for NP bioremediation processes. Proteomic data are available via ProteomeXchange with identifier PXDO04012.
Biological significance: To the best of our knowledge, this is the first report focussing on the effects of CdSe colloidal nanocrystals (CdSe NPs) on a marine strain of Pseudomonas fluorescens. CdSe NPs are extensively used in the industry of renewable energies and it is regrettably expected that these pollutants will sometime soon appear in the marine environment through surface runoff, urban effluents and rivers. Bacteria living in estuarine and coastal sediments will be among the first targets of these new pollutants. The pseudomonads are frequently found in these ecosystems. They are involved in several biogeochemical cycles and are known for their high resistance to pollutants. Consequently, this study focussing on the effects of CdSe NPs on the marine strain P. fluorescens BA3SM1 is highly relevant for several reasons. First, it aims at improving knowledge about the interactions between bacteria and NPs. This is fundamental to effectively use NPs against pathogenic bacteria. Secondly, in spite of CdSe NP interactions with the bacterial cells, the strain BA3SM1 can develop various strategies to counteract CdSe NP toxicity and ensure its growth. It exhibits interesting properties to sequester CdSe NPs and it retains its ability to form biofilm. The strain therefore appears as a promising agent for NP bioremediation thanks to biofiltration processes. Finally, this study shows that CdSe NPs of 8 nm in diameter cause a decrease in the secretion of siderophore pyoverdine, a secondary metabolite playing a key role in microbial ecology since it drives bacterial survival and competitiveness in ecosystems. Bacteria producing effective siderophores survive better in a Fe-deficient environment where they antagonize the growth of other microbes thought iron deprivation. Furthermore, siderophores are also employed as virulence factors in human pathogenic strains such as P. aeruginosa. Consequently, this study highlights that NPs can impact the secondary metabolism of bacteria with environmental and medical implications.
In addition, in this work, Data-Dependant Acquisition (DDA) provided state of the art Mass Spectrometry data by Spectral Counting and MS1 Label-Free. The combination of these two well-known proteomic techniques including manual validations strengthened the identification and quantification of regulated proteins. Moreover, numerous correlations between proteomic analyses and other observations (physiological, biochemical, microscopic) consolidated our interpretations. (C) 2016 Elsevier B.V. All rights reserved.
C1 [Poirier, Isabelle; Pallud, Marie; Bertrand, Martine] Conservatoire Natl Arts & Metiers, Inst Natl Sci & Tech Mer, F-50103 Octeville, France.
[Kuhn, Lauriane; Hammann, Philippe; Chicher, Johana] CNRS, Inst Biol Mol & Cellulaire, FRC1589, Plateforme Prote Strasbourg Esplanade, F-67084 Strasbourg, France.
[Demortiere, Arnaud; Mirvaux, Boris] Univ Picardie Jules Verne, CNRS, UMR 7314, Lab React & Chim Solides, F-80039 Amiens, France.
[Demortiere, Arnaud; Mirvaux, Boris] CNRS, FR 3459, RS2E, F-80039 Amiens, France.
[Caplat, Christelle] Normandie Univ, Inst Biol Fondamentale & Appl, UMR BOREA, UCBN,MNHN,UPMC,CNRS 7208,IRD 207, F-14032 Caen 5, France.
[Demortiere, Arnaud] Argonne Natl Lab, Ctr Nanoscale Mat, 9700 South Cass Ave, Argonne, IL 60439 USA.
RP Poirier, I (reprint author), Conservatoire Natl Arts & Metiers, Inst Natl Sci & Tech Mer, F-50103 Octeville, France.
EM isabelle.poirier@cnam.fr
FU Syndicat Mixte du Cotentin [Aval 2013/397]; Conseil Regional de
Basse-Normandie [2013 PCM 10 - NANOCEAN]
FX This work was financially supported by the "Syndicat Mixte du Cotentin"
(Aval 2013/397 - Des nanoparticules dans l'ocean) and the "Conseil
Regional de Basse-Normandie"(convention 2013 PCM 10 - NANOCEAN).
NR 73
TC 0
Z9 0
U1 18
U2 18
PU ELSEVIER SCIENCE BV
PI AMSTERDAM
PA PO BOX 211, 1000 AE AMSTERDAM, NETHERLANDS
SN 1874-3919
EI 1876-7737
J9 J PROTEOMICS
JI J. Proteomics
PD OCT 4
PY 2016
VL 148
BP 213
EP 227
DI 10.1016/j.jprot.2016.07.021
PG 15
WC Biochemical Research Methods
SC Biochemistry & Molecular Biology
GA DZ1LK
UT WOS:000385599700022
PM 27523480
ER
PT J
AU Montenegro-Burke, JR
Phommavongsay, T
Aisporna, AE
Huan, T
Rinehart, D
Forsberg, E
Poole, FL
Thorgersen, MP
Adams, MWW
Krantz, G
Fields, MW
Northen, TR
Robbins, PD
Niedernhofer, LJ
Lairson, L
Benton, HP
Siuzdak, G
AF Montenegro-Burke, J. Rafael
Phommavongsay, Thiery
Aisporna, Aries E.
Huan, Tao
Rinehart, Duane
Forsberg, Erica
Poole, Farris L.
Thorgersen, Michael P.
Adams, Michael W. W.
Krantz, Gregory
Fields, Matthew W.
Northen, Trent R.
Robbins, Paul D.
Niedernhofer, Laura J.
Lairson, Luke
Benton, H. Paul
Siuzdak, Gary
TI Smartphone Analytics: Mobilizing the Lab into the Cloud for OmicScale
Analyses
SO ANALYTICAL CHEMISTRY
LA English
DT Article
ID METABOLOMICS; METABOLISM; DATABASE; XCMS
AB Active data screening is an integral part of many scientific activities, and mobile technologies have greatly facilitated this process by minimizing the reliance on large hardware instrumentation. In order to meet with the increasingly growing field of metabolomics and heavy workload of data processing, we designed the first remote metabolomic data screening platform for mobile devices. Two mobile applications (apps), XCMS Mobile and METLIN Mobile, facilitate access to XCMS and METLIN, which are the most important components in the computer-based XCMS Online platforms. These mobile apps allow for the visualization and analysis of metabolic data throughout the entire analytical process. Specifically,: XCMS Mobile and METLIN Mobile provide the capabilities,for remote Monitoring of data processing, real time notifications for the data processing, visualization. and interactive analysis of processed data (eg., cloud: plots, principle,component analysis,. box plots; extracted ion chromatograms, and hierarchical cluster analysis), and database searching for metabolite identification. These apps, available on Apple iOS and Google Android operating systems, allow for the migration of metabolomic research onto mobile devices for better accessibility beyond direct instrument operation. The utility of XCMS While and METLIN Mobile functionalities was developed and is demonstrated here, through the metabolomic LC-MS analyses of stem cells, colon cancer, aging, and bacterial metabolism.
C1 [Montenegro-Burke, J. Rafael; Phommavongsay, Thiery; Aisporna, Aries E.; Huan, Tao; Rinehart, Duane; Forsberg, Erica; Benton, H. Paul; Siuzdak, Gary] Scripps Res Inst, Scripps Ctr Metabol, 10550 North Torrey Pines Rd, La Jolla, CA 92037 USA.
[Lairson, Luke] Scripps Res Inst, Dept Chem, 10550 North Torrey Pines Rd, La Jolla, CA 92037 USA.
[Robbins, Paul D.; Niedernhofer, Laura J.; Siuzdak, Gary] Scripps Res Inst, Dept Biol Chem, 10550 North Torrey Pines Rd, La Jolla, CA 92037 USA.
[Robbins, Paul D.; Niedernhofer, Laura J.; Siuzdak, Gary] Scripps Res Inst, Dept Mol Biol, 10550 North Torrey Pines Rd, La Jolla, CA 92037 USA.
[Robbins, Paul D.; Niedernhofer, Laura J.; Siuzdak, Gary] Scripps Res Inst, Dept Computat Biol, 10550 North Torrey Pines Rd, La Jolla, CA 92037 USA.
[Poole, Farris L.; Thorgersen, Michael P.; Adams, Michael W. W.] Univ Georgia, Dept Biochem & Mol Biol, Athens, GA 30602 USA.
[Krantz, Gregory; Fields, Matthew W.] Montana State Univ, Dept Microbiol & Immunol, 109 Lewis Hall, Bozeman, MT 59717 USA.
[Krantz, Gregory; Fields, Matthew W.] Montana State Univ, Ctr Biofilm Engn, 109 Lewis Hall, Bozeman, MT 59717 USA.
[Northen, Trent R.] Lawrence Berkeley Natl Lab, Div Life Sci, 1 Cyclotron Rd, Berkeley, CA 94720 USA.
[Robbins, Paul D.; Niedernhofer, Laura J.; Siuzdak, Gary] Scripps Res Inst Florida, Dept Metab, Jupiter, FL 33458 USA.
[Robbins, Paul D.; Niedernhofer, Laura J.; Siuzdak, Gary] Scripps Res Inst Florida, Dept Aging, Jupiter, FL 33458 USA.
RP Siuzdak, G (reprint author), Scripps Res Inst, Scripps Ctr Metabol, 10550 North Torrey Pines Rd, La Jolla, CA 92037 USA.; Siuzdak, G (reprint author), Scripps Res Inst, Dept Biol Chem, 10550 North Torrey Pines Rd, La Jolla, CA 92037 USA.; Siuzdak, G (reprint author), Scripps Res Inst, Dept Mol Biol, 10550 North Torrey Pines Rd, La Jolla, CA 92037 USA.; Siuzdak, G (reprint author), Scripps Res Inst, Dept Computat Biol, 10550 North Torrey Pines Rd, La Jolla, CA 92037 USA.; Siuzdak, G (reprint author), Scripps Res Inst Florida, Dept Metab, Jupiter, FL 33458 USA.; Siuzdak, G (reprint author), Scripps Res Inst Florida, Dept Aging, Jupiter, FL 33458 USA.
EM siuzdak@scripps.edu
OI Northen, Trent/0000-0001-8404-3259
FU Ecosystems and Networks Integrated with Genes and Molecular Assemblies;
Scientific Focus Area Program at Lawrence Berkeley National Laboratory
for the U.S. Department of Energy, Office of Science, Office of
Biological and Environmental Research [DE-AC02-05CH11231]; National
Institutes of Health (NIH) [R01 GMH4368, PO1 A1043376-02S1]
FX The authors thank the following for funding assistance: Ecosystems and
Networks Integrated with Genes and Molecular Assemblies
(http://enigma.lbl.gov), a Scientific Focus Area Program at Lawrence
Berkeley National Laboratory for the U.S. Department of Energy, Office
of Science, Office of Biological and Environmental Research under
contract number DE-AC02-05CH11231, and the National Institutes of Health
(NIH) grants R01 GMH4368 and PO1 A1043376-02S1.
NR 15
TC 1
Z9 1
U1 7
U2 7
PU AMER CHEMICAL SOC
PI WASHINGTON
PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA
SN 0003-2700
EI 1520-6882
J9 ANAL CHEM
JI Anal. Chem.
PD OCT 4
PY 2016
VL 88
IS 19
BP 9753
EP 9758
DI 10.1021/acs.analchem.6b02676
PG 6
WC Chemistry, Analytical
SC Chemistry
GA DY1GF
UT WOS:000384842200058
PM 27560777
ER
PT J
AU Yang, SI
George, GN
Lawrence, JR
Kaminskyj, SGW
Dynes, JJ
Lai, B
Pickering, IJ
AF Yang, Soo In
George, Graham N.
Lawrence, John R.
Kaminskyj, Susan G. W.
Dynes, James J.
Lai, Barry
Pickering, Ingrid J.
TI Multispecies Biofilms Transform Selenium Oxyanions into Elemental
Selenium Particles: Studies Using Combined Synchrotron X-ray
Fluorescence Imaging and Scanning Transmission X-ray Microscopy
SO ENVIRONMENTAL SCIENCE & TECHNOLOGY
LA English
DT Article
ID ABSORPTION SPECTROSCOPY; MICROBIAL BIOFILMS; RED SELENIUM; FOOD-CHAIN;
TOXICITY; NANOPARTICLES; SPECIATION; REDUCTION; BACTERIA; WATER
AB Selenium (Se) is an element of growing environmental concern, because low aqueous concentrations can lead to biomagnification through the aquatic food web. Biofilms, naturally occurring microbial consortia, play numerous important roles in the environment, especially in biogeochemical cycling of toxic elements in aquatic systems. The complexity of naturally forming multispecies biofilms presents challenges for characterization because conventional microscopic techniques require chemical and physical modifications of the sample. Here, multispecies biofilms biotransforming selenium oxyanions were characterized using Xray fluorescence imaging (XFI) and scanning trarismission X-ray microscopy (STXM) These complementary synchrotron techniques required minimal sample preparation and were applied correlatively to the same biofilm areas. Sub-micrometer XFI showed distributions of Se and endogenous metals, while Se Kedge X-ray absorption spectroscopy indicated.the presence of elemental Se (Se-0). Nanoscale carbon K-edge STXM revealed the distributions of microbial cells, extracellular polymeric substances (EPS), and lipids using the protein, saccharide, and lipid signatures, respectively, together with highly localized Se-0 using the Se L-iii edge. Transmission electron microscopy showed the electron-dense particle diameter to be 50-700 rim, suggesting Se-0 nanoparticles. The intimate association of Se-0 particles with protein and polysaccharide biofilm components has implications for the bioavailability of selenium in the environment.
C1 [Yang, Soo In; George, Graham N.; Pickering, Ingrid J.] Univ Saskatchewan, Dept Geol Sci, Saskatoon, SK S7N 5E2, Canada.
[Kaminskyj, Susan G. W.] Univ Saskatchewan, Dept Biol, Saskatoon, SK S7N 5E2, Canada.
[Lawrence, John R.] Environm Canada, Natl Hydrol Res Inst, Saskatoon, SK S7N 3H5, Canada.
[Dynes, James J.] Canadian Light Source, Saskatoon, SK S7N 2V3, Canada.
[Lai, Barry] Argonne Natl Lab, Adv Photon Source, 9700 S Cass Ave, Argonne, IL 60439 USA.
RP Pickering, IJ (reprint author), Univ Saskatchewan, Dept Geol Sci, Saskatoon, SK S7N 5E2, Canada.
EM ingrid.pickering@usask.ca
RI Pickering, Ingrid/A-4547-2013
FU Natural Sciences and Engineering Research Council of Canada (NSERC);
Saskatchewan Innovation and Science Fund; Environment Canada; Canada
Foundation for Innovation; NSERC; University of Saskatchewan; Government
of Saskatchewan; Western Economic Diversification Canada; National
Research Council Canada; Canadian Institutes of Health Research; U.S.
DOE [DE-AC02-06CH11357]
FX The authors thank members of the Ingrid J. Pickering/Graham N. George
group at the University of Saskatchewan and George Swerhone at
Environment Canada. This research is supported by a Natural Sciences and
Engineering Research Council of Canada (NSERC) Discovery Grant (to
Ingrid J. Pickering), Saskatchewan Innovation and Science Fund (to
Ingrid J. Pickering), and Environment Canada. Ingrid J. Pickering and
Graham N. George are Canada Research Chairs, and Soo In Yang is a
Canadian Institutes of Health Research Training grant in Health Research
Using Synchrotron Techniques (CIHR-THRUST) Fellow. The Canadian Light
Source is supported by the Canada Foundation for Innovation, NSERC, the
University of Saskatchewan, the Government of Saskatchewan, Western
Economic Diversification Canada, the National Research Council Canada,
and the Canadian Institutes of Health Research. Use of the Advanced
Photon Source, an Office of Science User Facility operated for the
United States Department of Energy (U.S. DOE) Office of Science by
Argonne National Laboratory, was supported by the U.S. DOE under
Contract DE-AC02-06CH11357.
NR 51
TC 1
Z9 1
U1 27
U2 27
PU AMER CHEMICAL SOC
PI WASHINGTON
PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA
SN 0013-936X
EI 1520-5851
J9 ENVIRON SCI TECHNOL
JI Environ. Sci. Technol.
PD OCT 4
PY 2016
VL 50
IS 19
BP 10343
EP 10350
DI 10.1021/acs.est.5b04529
PG 8
WC Engineering, Environmental; Environmental Sciences
SC Engineering; Environmental Sciences & Ecology
GA DY1GC
UT WOS:000384841900006
PM 26824614
ER
PT J
AU Willming, MM
Lilavois, CR
Barron, MG
Raimondo, S
AF Willming, Morgan M.
Lilavois, Crystal R.
Barron, Mace G.
Raimondo, Sandy
TI Acute Toxicity Prediction to Threatened and Endangered Species Using
Interspecies Correlation Estimation (ICE) Models
SO ENVIRONMENTAL SCIENCE & TECHNOLOGY
LA English
DT Article
ID SENSITIVITY DISTRIBUTIONS; CONTAMINANT SENSITIVITY; CHEMICALS; RISK
AB Evaluating contaminant sensitivity of threatened and endangered (listed) species and protectiveness of chemical regulations often depends on toxicity data for commonly tested surrogate species. The U.S. EPA's Internet application Web-ICE is a suite of Interspecies Correlation Estimation (ICE) models that can extrapolate species sensitivity to listed taxa using least-squares regressions of the sensitivity of a surrogate species and a predicted taxon (species, genus, or family). Web-ICE was expanded with new models that can predict toxicity to over 250 listed species. A case study was used to assess protectiveness of genus and family model estimates derived from either geometric mean or minimum taxa toxicity values for listed species. Models developed from the most sensitive value for each chemical were generally protective of the most sensitive species within predicted taxa, including listed species, and were more protective than geometric means models. ICE model estimates were compared to HC5 values derived from Species Sensitivity Distributions for the case study chemicals to assess protectiveness of the two approaches. ICE models provide robust toxicity predictions and can generate protective toxicity estimates for assessing contaminant risk to listed species.
C1 [Willming, Morgan M.] US EPA, Oak Ridge Inst Sci & Educ, Gulf Ecol Div, 1 Sabine Isl Dr, Gulf Breeze, FL 32561 USA.
[Lilavois, Crystal R.; Barron, Mace G.; Raimondo, Sandy] US EPA, Natl Hlth & Environm Effects Lab, Gulf Ecol Div, 1 Sabine Isl Dr, Gulf Breeze, FL 32561 USA.
RP Willming, MM (reprint author), US EPA, Oak Ridge Inst Sci & Educ, Gulf Ecol Div, 1 Sabine Isl Dr, Gulf Breeze, FL 32561 USA.
EM Willming.Morgan@epa.gov
NR 24
TC 2
Z9 2
U1 5
U2 5
PU AMER CHEMICAL SOC
PI WASHINGTON
PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA
SN 0013-936X
EI 1520-5851
J9 ENVIRON SCI TECHNOL
JI Environ. Sci. Technol.
PD OCT 4
PY 2016
VL 50
IS 19
BP 10700
EP 10707
DI 10.1021/acs.est.6b03009
PG 8
WC Engineering, Environmental; Environmental Sciences
SC Engineering; Environmental Sciences & Ecology
GA DY1GC
UT WOS:000384841900046
PM 27585402
ER
PT J
AU Maloubier, M
Shuh, DK
Minasian, SG
Pacold, JI
Solari, PL
Michel, H
Oberhaensli, FR
Bottein, Y
Monfort, M
Moulin, C
Den Auwer, C
AF Maloubier, Melody
Shuh, David K.
Minasian, Stefan G.
Pacold, Joseph I.
Solari, Pier-Lorenzo
Michel, Herve
Oberhaensli, Francois R.
Bottein, Yasmine
Monfort, Marguerite
Moulin, Christophe
Den Auwer, Christophe
TI How Do Radionuclides Accumulate in Marine Organisms? A Case Study of
Europium with Aplysina cavernicola
SO ENVIRONMENTAL SCIENCE & TECHNOLOGY
LA English
DT Article
ID RAY-ABSORPTION SPECTROSCOPY; LASER-INDUCED FLUORESCENCE; HEAVY-METALS;
CELLULAR-ORIGIN; BIOACCUMULATION; SPONGES; COMPLEXES; BIOMONITORS;
SPECIATION; POLLUTION
AB In the ocean, complex interactions between natural and anthropogenic radionuclides, seawater, and diverse marine biota provide a unique window through which to examine ecosystem and trophic transfer mechanisms in cases of accidental dissemination. The nature of interaction between radionuclides, the marine environment, and marine species is therefore essential for better understanding transfer mechanisms from the hydrosphere to the biosphere. Although data pertaining to the rate of global transfer are often available, little is known regarding the mechanism of environmental transport and uptake of heavy radionuclides by marine species. Among marine species, sponges are immobile active filter feeders and have been identified as hyperaccumulators of several heavy metals. We have selected the Mediterranean sponge Aplysina cavernicola as a model species for this study. Actinide elements are not the only source of radioactive release in cases of civilian nuclear events; however, their physicochemical transfer mechanisms to marine species remain largely unknown. We have targeted europium(III) as a representative of the trivalent actinides such as americium or curium. To unravel biological uptake mechanisms of europium in A cavernicola, we have combined radiometric (gamma) measurements with spectroscopic (time resolved laser-induced fluorescence spectroscopy, TRLIFS, and X-ray absorption near-edge structure, XANES) and imaging (transmission electron microscopy, TEM, and scanning transmission X-ray microscopy, STXM) techniques. We have observed that the colloids of NaEu(CO3)(2)center dot nH(2)O formed in seawater are taken up by A. cavernicola with no evidence that lethal dose has been reached in our working conditions. Spectroscopic results suggest that there is no change of speciation during uptake. Finally, TEM and STXM images recorded at different locations across a sponge cross section, together with differential cell separation, indicate the presence of europium particles (around 200 nm) mainly located in the skeleton and toward the outer surface of the sponge.
C1 [Maloubier, Melody; Michel, Herve; Den Auwer, Christophe] Univ Cote dAzur, Inst Chim Nice, F-06108 Nice, France.
[Maloubier, Melody; Michel, Herve; Den Auwer, Christophe] CNRS, F-06108 Nice, France.
[Maloubier, Melody; Monfort, Marguerite; Moulin, Christophe] CEA, Direct Applicat Mil, DIF, F-91297 Arpajon, France.
[Shuh, David K.; Minasian, Stefan G.; Pacold, Joseph I.] Lawrence Berkeley Natl Lab, Div Chem Sci, Berkeley, CA 94720 USA.
[Solari, Pier-Lorenzo] Synchrotron Soleil, BP 48, F-91192 Gif Sur Yvette, France.
[Oberhaensli, Francois R.; Bottein, Yasmine] IAEA, Monaco Environm Lab, 4 Quai Antoine Ier, Monaco 98000, Monaco.
RP Den Auwer, C (reprint author), Univ Cote dAzur, Inst Chim Nice, F-06108 Nice, France.; Den Auwer, C (reprint author), CNRS, F-06108 Nice, France.; Moulin, C (reprint author), CEA, Direct Applicat Mil, DIF, F-91297 Arpajon, France.
EM christophe.moulin@cea.fr; christophe.denauwer@unice.fr
FU DPN (Direction of Nuclear Propulsion) at Commissariat a l'Energie
Atomique; Direction des Applications Militaires (CEA/DAM); Centre
National de la Recherche Scientifique (CNRS)/Institut National de
Chimie; Government of the Principality of Monaco; Biosciences Heavy
Element Chemistry Program of the U.S. DOE at Lawrence Berkeley National
Laboratory (LBNL) [DE-AC02-05CH11231]; Office of Science, Office of
Basic Energy Sciences of the U.S. DOE [DE-AC02-05CH11231]; Interfacial
Molecular Sciences Program of the U.S. DOE at LBNL [DE-AC02-05CH11231]
FX This work was jointly financed by the DPN (Direction of Nuclear
Propulsion) at Commissariat a l'Energie Atomique, Direction des
Applications Militaires (CEA/DAM) and Centre National de la Recherche
Scientifique (CNRS)/Institut National de Chimie. The experimental work
on sponges was conducted under an internship at the IAEA Environment
Laboratories in Monaco. The International Atomic Energy Agency is
grateful to the Government of the Principality of Monaco for the support
provided to its Environment Laboratories. XAS experiments were performed
at the MARS beamline of Soleil Synchrotron, Gif sur Yvette, France. We
thank Professor O. P. Thomas and M. A. Tribalat for providing sponge
specimens and S. Pagnotta from the Microscopy Service (UNS) for TEM
analysis. D.K.S. and S.G.M. are supported by the Director, Office of
Science, Office of Basic Energy Sciences, Division of Chemical Sciences,
Geosciences, and Biosciences Heavy Element Chemistry Program of the U.S.
DOE at Lawrence Berkeley National Laboratory (LBNL) under Contract
DE-AC02-05CH11231. The Advanced Light Source (ALS) and TT were supported
by the Director, Office of Science, Office of Basic Energy Sciences, of
the U.S. DOE under Contract DE-AC02-05CH11231 at LBNL. Research at
bBeamline 11.0.2 at the ALS was supported by the Director, Office of
Science, Office of Basic Energy Sciences, Division of Chemical Sciences,
Geosciences, and Biosciences Condensed Phase and Interfacial Molecular
Sciences Program of the U.S. DOE at LBNL under Contract
DE-AC02-05CH11231.
NR 36
TC 0
Z9 0
U1 19
U2 19
PU AMER CHEMICAL SOC
PI WASHINGTON
PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA
SN 0013-936X
EI 1520-5851
J9 ENVIRON SCI TECHNOL
JI Environ. Sci. Technol.
PD OCT 4
PY 2016
VL 50
IS 19
BP 10730
EP 10738
DI 10.1021/acs.est.6b01896
PG 9
WC Engineering, Environmental; Environmental Sciences
SC Engineering; Environmental Sciences & Ecology
GA DY1GC
UT WOS:000384841900049
PM 27588898
ER
PT J
AU Ercan, NI
Stroeve, P
Tringe, JW
Faller, R
AF Ercan, Nazar Ileri
Stroeve, Pieter
Tringe, Joseph W.
Faller, Roland
TI Understanding the Interaction of Pluronics L61 and L64 with a DOPC Lipid
Bilayer: An Atomistic Molecular Dynamics Study
SO LANGMUIR
LA English
DT Article
ID PEO TRIBLOCK COPOLYMERS; LINEAR CONSTRAINT SOLVER; PARTICLE MESH EWALD;
X-RAY-SCATTERING; BLOCK-COPOLYMERS; POLY(ETHYLENE OXIDE);
AQUEOUS-SOLUTIONS; CELL-RESPONSE; FORCE-FIELD; SIMULATIONS
AB We investigate the interactions of Pluronics L61 and L64 with a dioleylphosphatidylcholine (DOPC) lipid bilayer by atomistic molecular dynamics simulations using the all-atom OPLS force field. Our results show that the initial configuration of the polymer with respect to the bilayer determines its final conformation within the bilayer. When the polymer is initially placed at the lipid/water interface, we observe partial insertion of the polymer in a U-shaped conformation. On the other hand, when the polymer is centered at the bilayer, it stabilizes to a transmembrane state, which facilitates water transport across the bilayer. We show that membrane thickness decreases while its fluidity increases in the presence of Pluronics. When the polymer concentration inside the bilayer is high, pore formation is initiated with L64. Our results show good agreement with existing experimental data and reveal that the hydrophilic/lipophilic balance of the polymer plays a critical role in the interaction mechanisms as well as in the dynamics of Pluronics with and within the bilayer.
C1 [Ercan, Nazar Ileri; Stroeve, Pieter; Faller, Roland] Univ Calif Davis, Dept Chem Engn, One Shields Ave, Davis, CA 95616 USA.
[Ercan, Nazar Ileri; Tringe, Joseph W.] Lawrence Livermore Natl Lab, 7000 East Ave, Livermore, CA 94551 USA.
[Ercan, Nazar Ileri] Bogazici Univ, Dept Chem Engn, TR-34342 Istanbul, Turkey.
RP Faller, R (reprint author), Univ Calif Davis, Dept Chem Engn, One Shields Ave, Davis, CA 95616 USA.
EM rfaller@ucdavis.edu
FU University of California Office of the President UCOP Lab Fee Program
[12-LR-237353]; U.S. Department of Energy by Lawrence Livermore National
Laboratory [DE-AC52-07NA27344]
FX This work was supported by a Grant from the University of California
Office of the President UCOP Lab Fee Program (Grant 12-LR-237353) and
was partially performed under the auspices of the U.S. Department of
Energy by Lawrence Livermore National Laboratory under Contract
DE-AC52-07NA27344. Computations were performed at LLNL Aztec and Sierra
massively parallel computers. Analysis were partially performed at
TUBITAK ULAKBIM, High Performance and Grid Computing Center (TRUBA
resources).
NR 60
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U1 5
U2 5
PU AMER CHEMICAL SOC
PI WASHINGTON
PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA
SN 0743-7463
J9 LANGMUIR
JI Langmuir
PD OCT 4
PY 2016
VL 32
IS 39
BP 10026
EP 10033
DI 10.1021/acs.langmuir.6b02360
PG 8
WC Chemistry, Multidisciplinary; Chemistry, Physical; Materials Science,
Multidisciplinary
SC Chemistry; Materials Science
GA DY1GD
UT WOS:000384842000013
ER
PT J
AU Berger, EL
Gao, J
Yuan, CP
Zhu, HX
AF Berger, Edmond L.
Gao, Jun
Yuan, C. -P.
Zhu, Hua Xing
TI NNLO QCD corrections to t-channel single top quark production and decay
SO PHYSICAL REVIEW D
LA English
DT Article
ID INELASTIC STRUCTURE FUNCTIONS; ORDER; SCATTERING; COLLISIONS; EVOLUTION;
LHC
AB We present a fully differential next-to-next-to-leading-order calculation of t-channel single top quark production and decay at the LHC under a narrow-width approximation and neglecting cross talk between incoming protons. We focus on the fiducial cross sections at 13 TeV, finding that the next-to-next-to-leading-order QCD corrections can reach the level of -6%. The scale variations are reduced to the level of a percent. Our results can be used to improve experimental acceptance estimates and the measurements of the single top quark production cross section and the top quark electroweak couplings.
C1 [Berger, Edmond L.; Gao, Jun] Argonne Natl Lab, High Energy Phys Div, 9700 S Cass Ave, Argonne, IL 60439 USA.
[Gao, Jun] Univ Calif Santa Barbara, Kavli Inst Theoret Phys, Santa Barbara, CA 93106 USA.
[Yuan, C. -P.] Michigan State Univ, Dept Phys & Astron, E Lansing, MI 48824 USA.
[Zhu, Hua Xing] MIT, Ctr Theoret Phys, Cambridge, MA 02139 USA.
RP Berger, EL; Gao, J (reprint author), Argonne Natl Lab, High Energy Phys Div, 9700 S Cass Ave, Argonne, IL 60439 USA.; Gao, J (reprint author), Univ Calif Santa Barbara, Kavli Inst Theoret Phys, Santa Barbara, CA 93106 USA.; Yuan, CP (reprint author), Michigan State Univ, Dept Phys & Astron, E Lansing, MI 48824 USA.; Zhu, HX (reprint author), MIT, Ctr Theoret Phys, Cambridge, MA 02139 USA.
EM berger@anl.gov; jgao@anl.gov; yuan@pa.msu.edu; zhuhx@mit.edu
RI Gao, Jun/C-9777-2017
FU U.S. Department of Energy [DE-AC02-06CH11357]; Office of Nuclear Physics
of the U.S. DOE [DE-SC0011090]; National Science Foundation [NSF
PHY-1125915, PHY-1417326]
FX Work at ANL is supported in part by the U.S. Department of Energy under
Contract No. DE-AC02-06CH11357. H. X. Z. was supported by the Office of
Nuclear Physics of the U.S. DOE under Contract No. DE-SC0011090. This
research was supported in part by the National Science Foundation under
Grants No. NSF PHY-1125915 and No. PHY-1417326. We thank Ze Long Liu for
cross-checking part of our results. We thank K. Melnikov and F. Caola
for providing numbers on inclusive cross sections for cross-checks. We
also thank T. Gehrmann, A. Papanastasiou, A. Signer, and Z. Sullivan for
useful conversations. We thank Southern Methodist University for the use
of the High Performance Computing facility ManeFrame.
NR 59
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U1 2
U2 2
PU AMER PHYSICAL SOC
PI COLLEGE PK
PA ONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA
SN 2470-0010
EI 2470-0029
J9 PHYS REV D
JI Phys. Rev. D
PD OCT 4
PY 2016
VL 94
IS 7
AR 071501
DI 10.1103/PhysRevD.94.071501
PG 6
WC Astronomy & Astrophysics; Physics, Particles & Fields
SC Astronomy & Astrophysics; Physics
GA DX7ZO
UT WOS:000384608100001
ER
PT J
AU Co, RT
D'Eramo, F
Hall, LJ
AF Co, Raymond T.
D'Eramo, Francesco
Hall, Lawrence J.
TI Supersymmetric axion grand unified theories and their predictions
SO PHYSICAL REVIEW D
LA English
DT Article
ID STRONG CP PROBLEM; INVISIBLE AXION; HARMLESS AXION; COSMOLOGY; SCALE;
PARTICLES
AB We introduce a class of unified supersymmetric axion theories with unified and Peccei-Quinn ( PQ) symmetries broken by the same set of fields at a scale similar to 2 x 10(16) GeV. Atypical domain wall number of order 30 leads to an axion decay constant f(a) of order 10(15) GeV. Inflation generates a large saxion condensate, giving a reheat temperature T-R below the QCD scale for supersymmetry breaking of order 1-10 TeV. Axion field oscillations commence in the saxion matter-dominated era near the QCD scale, and recent lattice computations of the temperature dependence of the axion mass in this era allow a controlled calculation of the axion dark matter abundance. The observed abundance can be successfully explained by an initial axion misalignment angle of order unity, theta(i) similar to 1. Ahighly correlated set of predictions is discussed for f(a), T-R, the supersymmetric Higgs mass parameter mu, the amount of dark radiation Delta N-eff, the proton decay rate Gamma(p -> e(+)pi(0)) isocurvature density perturbations and the B mode of the cosmic microwave background. The last two are particularly interesting when the energy scale of inflation is also of order 10(16) GeV.
C1 [Co, Raymond T.; Hall, Lawrence J.] Univ Calif Berkeley, Dept Phys, Berkeley Ctr Theoret Phys, Berkeley, CA 94720 USA.
[Co, Raymond T.; Hall, Lawrence J.] Lawrence Berkeley Natl Lab, Theoret Phys Grp, Berkeley, CA 94720 USA.
[D'Eramo, Francesco] Univ Calif Santa Cruz, Dept Phys, Santa Cruz, CA 95064 USA.
[D'Eramo, Francesco] Santa Cruz Inst Particle Phys, Santa Cruz, CA 95064 USA.
RP Co, RT (reprint author), Univ Calif Berkeley, Dept Phys, Berkeley Ctr Theoret Phys, Berkeley, CA 94720 USA.; Co, RT (reprint author), Lawrence Berkeley Natl Lab, Theoret Phys Grp, Berkeley, CA 94720 USA.
OI D'Eramo, Francesco/0000-0001-8499-7685; Co, Raymond/0000-0002-8395-7056
FU National Science Foundation [PHY-1002399, PHY-1316783]; National Science
Foundation Graduate Research Fellowship [DGE 1106400]; U.S. Department
of Energy [DE-SC0010107, DE-AC02-05CH11231]
FX We thank Michael Dine, Keisuke Harigaya and Hitoshi Murayama for useful
discussions. This work was supported in part by the Director, Office of
Science, Office of High Energy and Nuclear Physics, of the U.S.
Department of Energy under Contract No. DE-AC02-05CH11231 and by the
National Science Foundation under Grants No. PHY-1002399 and No.
PHY-1316783. R. C. is supported by the National Science Foundation
Graduate Research Fellowship under Grant No. DGE 1106400. F. D. is
supported by the U.S. Department of Energy Grant No. DE-SC0010107.
NR 40
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U1 0
U2 0
PU AMER PHYSICAL SOC
PI COLLEGE PK
PA ONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA
SN 2470-0010
EI 2470-0029
J9 PHYS REV D
JI Phys. Rev. D
PD OCT 4
PY 2016
VL 94
IS 7
AR 075001
DI 10.1103/PhysRevD.94.075001
PG 16
WC Astronomy & Astrophysics; Physics, Particles & Fields
SC Astronomy & Astrophysics; Physics
GA DX7ZO
UT WOS:000384608100005
ER
PT J
AU Migliori, A
Soderlind, P
Landa, A
Freibert, FJ
Maiorov, B
Ramshaw, BJ
Betts, JB
AF Migliori, Albert
Soderlind, Per
Landa, Alexander
Freibert, Franz J.
Maiorov, Boris
Ramshaw, B. J.
Betts, Jon B.
TI Origin of the multiple configurations that drive the response of
delta-plutonium's elastic moduli to temperature
SO PROCEEDINGS OF THE NATIONAL ACADEMY OF SCIENCES OF THE UNITED STATES OF
AMERICA
LA English
DT Article
DE δ plutonium; elastic moduli; thermal expansion; DFT
ID PU
AB The electronic and thermodynamic complexity of plutonium has resisted a fundamental understanding for this important elemental metal. A critical test of any theory is the unusual softening of the bulk modulus with increasing temperature, a result that is counterintuitive because no or very little change in the atomic volume is observed upon heating. This unexpected behavior has in the past been attributed to competing but never-observed electronic states with different bonding properties similar to the scenario with magnetic states in Invar alloys. Using the recent observation of plutonium dynamic magnetism, we construct a theory for plutonium that agrees with relevant measurements by using density-functional-theory (DFT) calculations with no free parameters to compute the effect of longitudinal spin fluctuations on the temperature dependence of the bulk moduli in delta-Pu. We show that the softening with temperature can be understood in terms of a continuous distribution of thermally activated spin fluctuations.
C1 [Migliori, Albert; Freibert, Franz J.; Maiorov, Boris; Ramshaw, B. J.; Betts, Jon B.] Los Alamos Natl Lab, Los Alamos, NM 87545 USA.
[Soderlind, Per; Landa, Alexander] Lawrence Livermore Natl Lab, Livermore, CA 94551 USA.
RP Migliori, A (reprint author), Los Alamos Natl Lab, Los Alamos, NM 87545 USA.
EM migliori@lanl.gov
FU Materials Science of Actinides, an Energy Frontier Research Center - US
Department of Energy (DOE), Office of Science, Basic Energy Sciences
[DE-SC0001089]; US DOE [DE-AC52-07NA27344]
FX We thank B. Sadigh for helpful discussions, and the Los Alamos Science
Campaigns and Laboratory Directed Research and Development. This work
was supported as part of the Materials Science of Actinides, an Energy
Frontier Research Center funded by the US Department of Energy (DOE),
Office of Science, Basic Energy Sciences under Award DE-SC0001089. The
detailed calculations were performed under the auspices of the US DOE by
Lawrence Livermore National Laboratory under Contract DE-AC52-07NA27344.
NR 21
TC 3
Z9 3
U1 18
U2 18
PU NATL ACAD SCIENCES
PI WASHINGTON
PA 2101 CONSTITUTION AVE NW, WASHINGTON, DC 20418 USA
SN 0027-8424
J9 P NATL ACAD SCI USA
JI Proc. Natl. Acad. Sci. U. S. A.
PD OCT 4
PY 2016
VL 113
IS 40
BP 11158
EP 11161
DI 10.1073/pnas.1609215113
PG 4
WC Multidisciplinary Sciences
SC Science & Technology - Other Topics
GA DX6XI
UT WOS:000384528900048
PM 27647904
ER
PT J
AU Shanker, S
Czako, R
Sapparapu, G
Alvarado, G
Viskovska, M
Sankaran, B
Atmar, RL
Crowe, JE
Estes, MK
Prasad, BVV
AF Shanker, Sreejesh
Czako, Rita
Sapparapu, Gopal
Alvarado, Gabriela
Viskovska, Maria
Sankaran, Banumathi
Atmar, Robert L.
Crowe, James E., Jr.
Estes, Mary K.
Prasad, B. V. Venkataram
TI Structural basis for norovirus neutralization by an HBGA blocking human
IgA antibody
SO PROCEEDINGS OF THE NATIONAL ACADEMY OF SCIENCES OF THE UNITED STATES OF
AMERICA
LA English
DT Article
DE norovirus; HBGA-blockade antibody; crystal structure; antibody
neutralization; viral entry
ID BLOOD GROUP ANTIGENS; NORWALK VIRUS-INFECTION; VACCINE DEVELOPMENT;
CRYSTALLOGRAPHIC STRUCTURE; BINDING SPECIFICITY; MONOCLONAL-ANTIBODY;
GII-4 NOROVIRUS; GASTROENTERITIS; SITE; RECOGNITION
AB Human noroviruses (HuNoVs) cause sporadic and epidemic gastroenteritis worldwide. They are classified into two major genogroups (GI and GII), with each genogroup further divided into multiple genotypes. Susceptibility to these viruses is influenced by genetically determined histo-blood group antigen (HBGA) expression. HBGAs function as cell attachment factors by binding to a surface-exposed region in the protruding (P) domain of the capsid protein. Sequence variations in this region that result in differential HBGA binding patterns and antigenicity are suggested to form a basis for strain diversification. Recent studies show that serum antibodies that block HBGA binding correlate with protection against illness. Although genogroup-dependent variation in HBGA binding specificity is structurally well characterized, an understanding of how antibodies block HBGA binding and how genotypic variations affect such blockade is lacking. Our crystallographic studies of the GI. 1 P domain in complex with the Fab fragment of a human IgA monoclonal antibody (IgA 5I2) with HBGA blocking activity show that the antibody recognizes a conformational epitope formed by two surface-exposed loop clusters in the P domain. The antibody engulfs the HBGA binding site but does not affect its structural integrity. An unusual feature of the antigen recognition by IgA 5I2 is the predominant involvement of the CDR light chain 1 in contrast to the commonly observed CDR heavy chain 3, providing a unique perspective into antibody diversity in antigen recognition. Identification of the antigenic site in the P domain shows how genotypic variations might allow escape from antibody neutralization and exemplifies the interplay between antigenicity and HBGA specificity in HuNoV evolution.
C1 [Shanker, Sreejesh; Viskovska, Maria; Prasad, B. V. Venkataram] Baylor Coll Med, Verna & Marrs McLean Dept Biochem & Mol Biol, Houston, TX 77030 USA.
[Czako, Rita; Atmar, Robert L.; Estes, Mary K.; Prasad, B. V. Venkataram] Baylor Coll Med, Dept Mol Virol & Microbiol, Houston, TX 77030 USA.
[Sapparapu, Gopal; Crowe, James E., Jr.] Vanderbilt Univ, Med Ctr, Dept Pediat, Nashville, TN 37232 USA.
[Alvarado, Gabriela; Crowe, James E., Jr.] Vanderbilt Univ, Med Ctr, Dept Pathol Microbiol & Immunol, Nashville, TN 37232 USA.
[Sankaran, Banumathi] Lawrence Berkeley Lab, Berkeley Ctr Struct Biol Mol Biophys & Integrated, Berkeley, CA 94720 USA.
[Atmar, Robert L.; Estes, Mary K.] Baylor Coll Med, Dept Med, Houston, TX 77030 USA.
RP Prasad, BVV (reprint author), Baylor Coll Med, Verna & Marrs McLean Dept Biochem & Mol Biol, Houston, TX 77030 USA.; Estes, MK; Prasad, BVV (reprint author), Baylor Coll Med, Dept Mol Virol & Microbiol, Houston, TX 77030 USA.; Estes, MK (reprint author), Baylor Coll Med, Dept Med, Houston, TX 77030 USA.
EM mestes@bcm.edu; vprasad@bcm.edu
OI Crowe, James/0000-0002-0049-1079; Sapparapu, Gopal/0000-0001-9670-1757
FU Public Health Service Grants [NIH P01 AI057788, NIH P30 DK56338, P30
CA125123]; Robert Welch Foundation Grant [Q1292]; Agriculture and Food
Research Initiative Competitive Grant US Department of Agriculture
National Institute of Food and Agriculture [2011-68003-30395]; John S.
Dunn Research Foundation
FX We acknowledge the use of the synchrotron beamlines at the Advanced
Light Source (5.0.1) (Berkeley, CA) for diffraction data collection and
thank their staff for excellent help. This research was funded by Public
Health Service Grants NIH P01 AI057788, NIH P30 DK56338, and P30
CA125123; Robert Welch Foundation Grant Q1292; Agriculture and Food
Research Initiative Competitive Grant 2011-68003-30395 from the US
Department of Agriculture National Institute of Food and Agriculture;
and the John S. Dunn Research Foundation.
NR 62
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U1 6
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PU NATL ACAD SCIENCES
PI WASHINGTON
PA 2101 CONSTITUTION AVE NW, WASHINGTON, DC 20418 USA
SN 0027-8424
J9 P NATL ACAD SCI USA
JI Proc. Natl. Acad. Sci. U. S. A.
PD OCT 4
PY 2016
VL 113
IS 40
BP E5830
EP E5837
DI 10.1073/pnas.1609990113
PG 8
WC Multidisciplinary Sciences
SC Science & Technology - Other Topics
GA DX6XI
UT WOS:000384528900009
PM 27647885
ER
PT J
AU Varman, AM
He, L
Follenfant, R
Wu, WH
Wemmer, S
Wrobel, SA
Tang, YJJ
Singh, S
AF Varman, Arul M.
He, Lian
Follenfant, Rhiannon
Wu, Weihua
Wemmer, Sarah
Wrobel, Steven A.
Tang, Yinjie J.
Singh, Seema
TI Decoding how a soil bacterium extracts building blocks and metabolic
energy from ligninolysis provides road map for lignin valorization
SO PROCEEDINGS OF THE NATIONAL ACADEMY OF SCIENCES OF THE UNITED STATES OF
AMERICA
LA English
DT Article
DE C-13-MFA; fingerprinting; gluconeogenesis; NADPH; lignin
ID SPHINGOMONAS-PAUCIMOBILIS SYK-6; DEPENDENT O-DEMETHYLASE; WOOD-LJUNGDAHL
PATHWAY; ONE-CARBON METABOLISM; C-13 FLUX ANALYSIS; BIOFUEL PRODUCTION;
LIGNOCELLULOSIC BIOMASS; ARABIDOPSIS-THALIANA; NEUROSPORA-CRASSA;
ESCHERICHIA-COLI
AB Sphingobium sp. SYK-6 is a soil bacterium boasting a well-studied ligninolytic pathway and the potential for development into a microbial chassis for lignin valorization. An improved understanding of its metabolism will help researchers in the engineering of SYK-6 for the production of value-added chemicals through lignin valorization. We used C-13-fingerprinting, C-13 metabolic flux analysis (C-13-MFA), and RNA-sequencing differential expression analysis to uncover the following metabolic traits: (i) SYK-6 prefers alkaline conditions, making it an efficient host for the consolidated bioprocessing of lignin, and it also lacks the ability to metabolize sugars or organic acids; (ii) the CO2 release (i. e., carbon loss) from the ligninolysis-based metabolism of SYK-6 is significantly greater than the CO2 release from the sugar-basedmetabolism of Escherichia coli; (iii) the vanillin catabolic pathway (which is the converging point of majority of the lignin catabolic pathways) is coupled with the tetrahydrofolate-dependent C1 pathway that is essential for the biosynthesis of serine, histidine, and methionine; (iv) catabolic end products of lignin (pyruvate and oxaloacetate) must enter the tricarboxylic acid (TCA) cycle first and then use phosphoenolpyruvate carboxykinase to initiate gluconeogenesis; and (v) C-13-MFA together with RNA-sequencing differential expression analysis establishes the vanillin catabolic pathway as the major contributor of NAD(P) H synthesis. Therefore, the vanillin catabolic pathway is essential for SYK-6 to obtain sufficient reducing equivalents for its healthy growth; cosubstrate experiments support this finding. This unique energy feature of SYK-6 is particularly interesting because most heterotrophs rely on the transhydrogenase, the TCA cycle, and the oxidative pentose phosphate pathway to obtain NADPH.
C1 [Varman, Arul M.; Follenfant, Rhiannon; Wu, Weihua; Wemmer, Sarah; Wrobel, Steven A.; Singh, Seema] Sandia Natl Labs, Biomass Sci & Convers Technol Dept, Livermore, CA 94550 USA.
[He, Lian; Tang, Yinjie J.] Washington Univ, Dept Energy Environm & Chem Engn, St Louis, MO 63130 USA.
[Singh, Seema] Univ Minnesota, Dept Bioprod & Biosyst Engn, St Paul, MN 55108 USA.
RP Singh, S (reprint author), Sandia Natl Labs, Biomass Sci & Convers Technol Dept, Livermore, CA 94550 USA.; Singh, S (reprint author), Univ Minnesota, Dept Bioprod & Biosyst Engn, St Paul, MN 55108 USA.
EM seesing@sandia.gov
FU Laboratory Directed Research and Development Program of Sandia National
Laboratories [16-0758]; US Department of Energy's National Nuclear
Security Administration [DE-AC04-94AL85000]; NSF [DBI 1356669]
FX We thank Joint BioEnergy Institute for the SYK6 strain, Yu Yi for the
technical discussions, and Whitney Hollinshead for her help with the
GCMS. This project was supported by Laboratory Directed Research and
Development Program 16-0758 of Sandia National Laboratories to Principal
Investigator S.S. Sandia is a multiprogram laboratory operated by Sandia
Corporation, a Lockheed Martin Company, for the US Department of
Energy's National Nuclear Security Administration under Contract
DE-AC04-94AL85000. L.H. was supported by NSF Grant DBI 1356669.
NR 60
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U1 13
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PU NATL ACAD SCIENCES
PI WASHINGTON
PA 2101 CONSTITUTION AVE NW, WASHINGTON, DC 20418 USA
SN 0027-8424
J9 P NATL ACAD SCI USA
JI Proc. Natl. Acad. Sci. U. S. A.
PD OCT 4
PY 2016
VL 113
IS 40
BP E5802
EP E5811
DI 10.1073/pnas.1606043113
PG 10
WC Multidisciplinary Sciences
SC Science & Technology - Other Topics
GA DX6XI
UT WOS:000384528900006
PM 27634497
ER
PT J
AU Kalluri, UC
Payyavula, RS
Labbe, JL
Engle, N
Bali, G
Jawdy, SS
Sykes, RW
Davis, M
Ragauskas, A
Tuskan, GA
Tschaplinski, TJ
AF Kalluri, Udaya C.
Payyavula, Raja S.
Labbe, Jessy L.
Engle, Nancy
Bali, Garima
Jawdy, Sara S.
Sykes, Robert W.
Davis, Mark
Ragauskas, Arthur
Tuskan, Gerald A.
Tschaplinski, Timothy J.
TI Down-Regulation of KORRIGAN-Like Endo-beta-1,4-Glucanase Genes Impacts
Carbon Partitioning, Mycorrhizal Colonization and Biomass Production in
Populus
SO FRONTIERS IN PLANT SCIENCE
LA English
DT Article
DE plant cell wall; endo-beta-1,4-glucanase; carbon partitioning and
allocation; cellulose; biomass; mycorrhiza; microbe; Populus
ID SECONDARY CELL-WALL; OSMOTIC-STRESS TOLERANCE; ARABIDOPSIS-THALIANA;
TRICHODERMA-HARZIANUM; DEFENSE RESPONSES; LACCARIA-BICOLOR; CELLULOSE;
TRICHOCARPA; GENOME; SPECTROSCOPY
AB A greater understanding of the genetic regulation of plant cell wall remodeling and the impact of modified cell walls on plant performance is important for the development of sustainable biofuel crops. Here, we studied the impact of down-regulating KORRIGAN-like cell wall biosynthesis genes, belonging to the endo-beta-1,4-glucanase gene family, on Populus growth, metabolism and the ability to interact with symbiotic microbes. The reductions in cellulose content and lignin syringyl-to-guaiacyl unit ratio, and increase in cellulose crystallinity of cell walls of PdKOR RNAi plants corroborated the functional role of PdKOR in cell wall biosynthesis. Altered metabolism and reduced growth characteristics of RNAi plants revealed new implications on carbon allocation and partitioning. The distinctive metabolome phenotype comprised of a higher phenolic and salicylic acid content, and reduced lignin, shikimic acid and maleic acid content relative to control. Plant sustainability implications of modified cell walls on beneficial plant-microbe interactions were explored via co-culture with an ectomycorrhizal fungus, Laccaria bicolor. A significant increase in the mycorrhization rate was observed in transgenic plants, leading to measurable beneficial growth effects. These findings present new evidence for functional interconnectedness of cellulose biosynthesis pathway, metabolism and mycorrhizal association in plants, and further emphasize the consideration of the sustainability implications of plant trait improvement efforts.
C1 [Kalluri, Udaya C.; Payyavula, Raja S.; Labbe, Jessy L.; Engle, Nancy; Jawdy, Sara S.; Tuskan, Gerald A.; Tschaplinski, Timothy J.] Oak Ridge Natl Lab, BioEnergy Sci, Oak Ridge, TN 37831 USA.
[Kalluri, Udaya C.; Payyavula, Raja S.; Labbe, Jessy L.; Engle, Nancy; Jawdy, Sara S.; Tuskan, Gerald A.; Tschaplinski, Timothy J.] Oak Ridge Natl Lab, Biosci Div, Oak Ridge, TN 37831 USA.
[Bali, Garima] Georgia Inst Technol, Inst Paper Sci & Technol, BioEnergy Sci Ctr, Sch Chem & Biochem, Atlanta, GA 30332 USA.
[Sykes, Robert W.; Davis, Mark] Natl Renewable Energy Lab, Biosci Ctr, Golden, CO USA.
[Ragauskas, Arthur] Univ Tennessee, Oak Ridge Natl Lab, Dept Chem & Biomol Engn, Knoxville, TN USA.
[Ragauskas, Arthur] Univ Tennessee, Dept Forestry Wildlife & Fisheries, Knoxville, TN USA.
RP Kalluri, UC (reprint author), Oak Ridge Natl Lab, BioEnergy Sci, Oak Ridge, TN 37831 USA.; Kalluri, UC (reprint author), Oak Ridge Natl Lab, Biosci Div, Oak Ridge, TN 37831 USA.
EM kalluriudayc@oml.gov
FU U.S. Department of Energy, Office of Science, Biological and
Environmental Research; Plant Microbe Interfaces (PMI) projects; Office
of Biological and Environmental Research in the DOE Office of Science;
U.S. Department of Energy [DE-AC05-00OR22725]
FX This research was supported by funding from U.S. Department of Energy,
Office of Science, Biological and Environmental Research to the
BioEnergy Science Center (BESC) and Plant Microbe Interfaces (PMI)
projects. BESC is a U.S. DOE Energy Bioenergy Research Center supported
by the Office of Biological and Environmental Research in the DOE Office
of Science. Oak Ridge National Laboratory is managed by UT-Battelle, LLC
for the U.S. Department of Energy: under Contract Number
DE-AC05-00OR22725. Oak Ridge National Laboratory is managed by
UT-Battelle, LLC for the DOE under Contract Number DE-AC05-00OR22725.
NR 64
TC 0
Z9 0
U1 13
U2 13
PU FRONTIERS MEDIA SA
PI LAUSANNE
PA PO BOX 110, EPFL INNOVATION PARK, BUILDING I, LAUSANNE, 1015,
SWITZERLAND
SN 1664-462X
J9 FRONT PLANT SCI
JI Front. Plant Sci.
PD OCT 4
PY 2016
VL 7
AR 1455
DI 10.3389/fpls.2016.01455
PG 12
WC Plant Sciences
SC Plant Sciences
GA DX9CT
UT WOS:000384691800001
PM 27757116
ER
PT J
AU Hruszkewycz, SO
Zhang, Q
Holt, MV
Highland, MJ
Evans, PG
Fuoss, PH
AF Hruszkewycz, S. O.
Zhang, Q.
Holt, M. V.
Highland, M. J.
Evans, P. G.
Fuoss, P. H.
TI Structural sensitivity of x-ray Bragg projection ptychography to domain
patterns in epitaxial thin films
SO PHYSICAL REVIEW A
LA English
DT Article
ID DIFFRACTION; SUPERLATTICES; MICROSCOPY; DISTORTIONS
AB Bragg projection ptychography (BPP) is a coherent diffraction imaging technique capable of mapping the spatial distribution of the Bragg structure factor in nanostructured thin films. Here, we show that, because these images are projections, the structural sensitivity of the resulting images depends on the film thickness and the aspect ratio and orientation of the features of interest and that image interpretation depends on these factors. We model changes in contrast in the BPP reconstructions of simulated PbTiO3 ferroelectric thin films with meandering 180 degrees stripe domains as a function of film thickness, discuss their origin, and comment on the implication of these factors on the design of BPP experiments of general nanostructured films.
C1 [Hruszkewycz, S. O.; Highland, M. J.; Fuoss, P. H.] Argonne Natl Lab, Div Mat Sci, 9700 S Cass Ave, Argonne, IL 60439 USA.
[Zhang, Q.; Evans, P. G.] Univ Wisconsin, Dept Mat Sci & Engn, Madison, WI 53706 USA.
[Holt, M. V.] Argonne Natl Lab, Ctr Nanoscale Mat, 9700 S Cass Ave, Argonne, IL 60439 USA.
[Fuoss, P. H.] Argonne Natl Lab, Adv Photon Source, Argonne, IL 60439 USA.
RP Hruszkewycz, SO (reprint author), Argonne Natl Lab, Div Mat Sci, 9700 S Cass Ave, Argonne, IL 60439 USA.
EM shrus@anl.gov
RI Evans, Paul/A-9260-2009
OI Evans, Paul/0000-0003-0421-6792
FU U.S. Department of Energy, Office of Science, Basic Energy Sciences,
Materials Sciences and Engineering Division; U.S. Department of Energy,
Basic Energy Sciences, Materials Sciences and Engineering Division
[DE-FG02-04ER46147]; U.S. Department of Energy, Office of Science,
Office of Basic Energy Sciences [DE-AC02-06CH11357]
FX Ptychographic simulations and generation of reconstructions were
supported by the U.S. Department of Energy, Office of Science, Basic
Energy Sciences, Materials Sciences and Engineering Division. Geometric
algorithms for the simulation of the nanodomain arrangement were
developed at University of Wisconsin-Madison under support from U.S.
Department of Energy, Basic Energy Sciences, Materials Sciences and
Engineering Division under Contract No. DE-FG02-04ER46147. Use of the
Center for Nanoscale Materials was supported by the U.S. Department of
Energy, Office of Science, Office of Basic Energy Sciences, under
Contract No. DE-AC02-06CH11357.
NR 31
TC 1
Z9 1
U1 17
U2 17
PU AMER PHYSICAL SOC
PI COLLEGE PK
PA ONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA
SN 2469-9926
EI 2469-9934
J9 PHYS REV A
JI Phys. Rev. A
PD OCT 4
PY 2016
VL 94
IS 4
AR 043803
DI 10.1103/PhysRevA.94.043803
PG 6
WC Optics; Physics, Atomic, Molecular & Chemical
SC Optics; Physics
GA DX7XQ
UT WOS:000384603100008
ER
PT J
AU Porter, DG
Senn, MS
Khalyavin, DD
Cortese, A
Waterfield-Price, N
Radaelli, PG
Manuel, P
zur-Loye, HC
Mazzoli, C
Bombardi, A
AF Porter, D. G.
Senn, M. S.
Khalyavin, D. D.
Cortese, A.
Waterfield-Price, N.
Radaelli, P. G.
Manuel, P.
zur-Loye, H. -C.
Mazzoli, C.
Bombardi, A.
TI Magnetostriction-driven ground-state stabilization in 2H perovskites
SO PHYSICAL REVIEW B
LA English
DT Article
ID 2H-PEROVSKITE RELATED OXIDES; MAGNETIC-PROPERTIES; CRYSTAL-STRUCTURE;
TEMPERATURE; GROWTH
AB The magnetic ground state of Sr(3)ARuO(6), with A = (Li, Na), is studied using neutron diffraction, resonant x-ray scattering, and laboratory characterization measurements of high-quality crystals. Combining these results allows us to observe the onset of long-range magnetic order and distinguish the symmetrically allowed magnetic models, identifying in-plane antiferromagnetic moments and a small ferromagnetic component along the c axis. While the existence of magnetic domains masks the particular in-plane direction of the moments, it has been possible to elucidate the ground state using symmetry considerations. We find that due to the lack of local anisotropy, antisymmetric exchange interactions control the magnetic order, first through structural distortions that couple to in-plane antiferromagnetic moments and second through a high-order magnetoelastic coupling that lifts the degeneracy of the in-plane moments. The symmetry considerations used to rationalize the magnetic ground state are very general and will apply to many systems in this family, such as Ca(3)ARuO(6), with A = (Li,Na), and Ca3LiOsO6 whose magnetic ground states are still not completely understood.
C1 [Porter, D. G.; Senn, M. S.; Waterfield-Price, N.; Bombardi, A.] Diamond Light Source Ltd, Harwell Sci & Innovat Campus, Didcot OX11 0DE, Oxon, England.
[Senn, M. S.] Univ Oxford, Inorgan Chem Lab, South Parks Rd, Oxford OX1 3QR, England.
[Khalyavin, D. D.; Manuel, P.] STFC, Rutherford Appleton Lab, ISIS Facil, Didcot OX11 0QX, Oxon, England.
[Cortese, A.; zur-Loye, H. -C.] Univ South Carolina, Dept Chem & Biochem, Columbia, SC 29208 USA.
[Waterfield-Price, N.; Radaelli, P. G.; Bombardi, A.] Univ Oxford, Dept Phys, Parks Rd, Oxford OX1 3PU, England.
[Mazzoli, C.] Politecn Milan, Unita CNISM, Dip Fis 6, Piazza Leonardo Da Vinci 32, I-20133 Milan, Italy.
[Mazzoli, C.] Brookhaven Natl Lab, Natl Synchrotron Light Source 2, Upton, NY 11973 USA.
RP Porter, DG (reprint author), Diamond Light Source Ltd, Harwell Sci & Innovat Campus, Didcot OX11 0DE, Oxon, England.
EM dan.porter@diamond.ac.uk
RI Khalyavin, Dmitry/E-4335-2017; Radaelli, Paolo/C-2952-2011;
OI Khalyavin, Dmitry/0000-0002-6724-7695; Radaelli,
Paolo/0000-0002-6717-035X; Waterfield Price, Noah/0000-0002-7097-4383;
Porter, Daniel/0000-0002-9397-7835
FU TUMOCS; European Union [645660]; NSF [DMR-1301757]
FX We acknowledge Diamond Light Source for time on Beamline I16 under
Proposal No. 9409. We acknowledge ISIS for time on the instrument Wish
under Proposal No. 1520273. Work at ISIS was supported by project
TUMOCS. This project has received funding from the European Union's
Horizon 2020 research and innovation programme under the Marie
Sklodowska-Curie Grant Agreement No. 645660. H.z.L. and A.C. acknowledge
support from the NSF via Award No. DMR-1301757. C.M. thanks Diamond
Light Source for their hospitality during this work. Images of atomic
structures were created using the computer program VESTA, by K. Momma
and F. Izumi [30].
NR 33
TC 0
Z9 0
U1 6
U2 6
PU AMER PHYSICAL SOC
PI COLLEGE PK
PA ONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA
SN 2469-9950
EI 2469-9969
J9 PHYS REV B
JI Phys. Rev. B
PD OCT 4
PY 2016
VL 94
IS 13
AR 134404
DI 10.1103/PhysRevB.94.134404
PG 11
WC Physics, Condensed Matter
SC Physics
GA DX7XZ
UT WOS:000384604000002
ER
PT J
AU Johns, L
Mina, M
Cirigliano, V
Paris, MW
Fuller, GM
AF Johns, Lucas
Mina, Mattia
Cirigliano, Vincenzo
Paris, Mark W.
Fuller, George M.
TI Neutrino flavor transformation in the lepton-asymmetric universe
SO PHYSICAL REVIEW D
LA English
DT Article
ID NONEQUILIBRIUM CORRECTIONS; MASSLESS NEUTRINOS; DARK-MATTER; X-RAY;
OSCILLATIONS; NUMBER; SPECTRA; NUCLEOSYNTHESIS; VIOLATION; PHYSICS
AB We investigate neutrino flavor transformation in the early Universe in the presence of a lepton asymmetry, focusing on a two-flavor system with 1-3 mixing parameters. We identify five distinct regimes that emerge in an approximate treatment neglecting collisions as the initial lepton asymmetry at high temperature is varied from values comparable to current constraints on the lepton number down to values at which the neutrino-neutrino forward-scattering potential is negligible. The characteristic phenomena occurring in these regimes are (1) large synchronized oscillations, (2) minimal flavor transformation, (3) asymmetric (nu- or (nu) over bar -only) MSW, (4) partial MSW, and (5) symmetric MSW. We examine our numerical results in the framework of adiabaticity, and we illustrate how they are modified by collisional damping. Finally, we point out the existence of matter-neutrino resonances in the early Universe and show that they suffer from nonadiabaticity.
C1 [Johns, Lucas; Fuller, George M.] Univ Calif San Diego, Dept Phys, La Jolla, CA 92093 USA.
[Johns, Lucas; Mina, Mattia; Cirigliano, Vincenzo; Paris, Mark W.] Los Alamos Natl Lab, Theoret Div, Los Alamos, NM 87545 USA.
[Mina, Mattia] Univ Turin, Dept Phys, Via P Giuria 1, I-10125 Turin, Italy.
RP Johns, L (reprint author), Univ Calif San Diego, Dept Phys, La Jolla, CA 92093 USA.; Johns, L (reprint author), Los Alamos Natl Lab, Theoret Div, Los Alamos, NM 87545 USA.
EM ljohns@physics.ucsd.edu
OI Paris, Mark/0000-0003-0471-7896
FU NSF at UC San Diego [PHY-1307372]; Los Alamos National Laboratory
Institute for Geophysics, Space Sciences and Signatures [257842]; Los
Alamos National Laboratory Institutional Computing Program, under U.S.
Department of Energy National Nuclear Security Administration
[DE-AC52-06NA25396]; Los Alamos National Laboratory LDRD Program; U.S.
Department of Energy Office of Science Graduate Student Research (SCGSR)
Program
FX We thank Brad Keister, Chad Kishimoto, and Amol Patwardhan for helpful
conversations. This work was supported by NSF Grant No. PHY-1307372 at
UC San Diego; by the Los Alamos National Laboratory Institute for
Geophysics, Space Sciences and Signatures Contract No. 257842; by the
Los Alamos National Laboratory Institutional Computing Program, under
U.S. Department of Energy National Nuclear Security Administration Award
No. DE-AC52-06NA25396; by the Los Alamos National Laboratory LDRD
Program; and by the U.S. Department of Energy Office of Science Graduate
Student Research (SCGSR) Program.
NR 105
TC 4
Z9 4
U1 1
U2 1
PU AMER PHYSICAL SOC
PI COLLEGE PK
PA ONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA
SN 2470-0010
EI 2470-0029
J9 PHYS REV D
JI Phys. Rev. D
PD OCT 4
PY 2016
VL 94
IS 8
AR 083505
DI 10.1103/PhysRevD.94.083505
PG 18
WC Astronomy & Astrophysics; Physics, Particles & Fields
SC Astronomy & Astrophysics; Physics
GA DX8AD
UT WOS:000384609600006
ER
PT J
AU Du, JL
Fang, Y
Fu, EG
Ding, X
Yu, KY
Wang, YG
Wang, YQ
Baldwin, JK
Wang, PP
Bai, Q
AF Du, J. L.
Fang, Y.
Fu, E. G.
Ding, X.
Yu, K. Y.
Wang, Y. G.
Wang, Y. Q.
Baldwin, J. K.
Wang, P. P.
Bai, Q.
TI What determines the interfacial configuration of Nb/Al2O3 and Nb/MgO
interface
SO SCIENTIFIC REPORTS
LA English
DT Article
ID TRANSMISSION ELECTRON-MICROSCOPY; EPITAXIAL NB-AL2O3 INTERFACES;
HETEROPHASE INTERFACE; MECHANICAL-PROPERTIES; MISFIT DISLOCATIONS;
ATOMIC-STRUCTURE; SPUTTERED CU/V; NB FILMS; STEELS; SAPPHIRE
AB Nb films are deposited on single crystal Al2O3 (11 (2) over bar0) and MgO(111) substrates by e-beam evaporation technique. Structure of Nb films and orientation relationships (ORs) of Nb/Al2O3 and Nb/MgO interface are studied and compared by the combination of experiments and simulations. The experiments show that the Nb films obtain strong (110) texture, and the Nb film on Al2O3(11 (2) over bar0) substrate shows a higher crystalline quality than that on MgO(111) substrate. First principle calculations show that both the lattice mismatch and the strength of interface bonding play major roles in determining the crystalline perfection of Nb films and ORs between Nb films and single crystal ceramic substrates. The fundamental mechanisms for forming the interfacial configuration in terms of the lattice mismatch and the strength of interface bonding are discussed.
C1 [Du, J. L.; Fu, E. G.; Wang, Y. G.; Wang, P. P.; Bai, Q.] Peking Univ, Sch Phys, State Key Lab Nucl Phys & Technol, Beijing 100871, Peoples R China.
[Fang, Y.; Ding, X.] Xi An Jiao Tong Univ, State Key Lab Mech Behav Mat, Xian 710049, Peoples R China.
[Yu, K. Y.] China Univ Petr, Dept Mat Sci & Engn, Beijing 102249, Peoples R China.
[Wang, Y. Q.; Baldwin, J. K.] Los Alamos Natl Lab, Expt Phys Sci Directorate, Los Alamos, NM 87544 USA.
RP Fu, EG (reprint author), Peking Univ, Sch Phys, State Key Lab Nucl Phys & Technol, Beijing 100871, Peoples R China.; Ding, X (reprint author), Xi An Jiao Tong Univ, State Key Lab Mech Behav Mat, Xian 710049, Peoples R China.; Yu, KY (reprint author), China Univ Petr, Dept Mat Sci & Engn, Beijing 102249, Peoples R China.
EM efu@pku.edu.cn; dingxd@mail.xjtu.edu.cn; kyyu@cup.edu.cn
FU Electron Microscopy Laboratory of Peking University; ITER from Ministry
of Science and Technology [2015GB121004]; Natural Science Foundation of
China [11375018, 11528508]; Recruitment Program of Global Youth Experts
in China; Instrumental Analysis Fund of Peking University; NSFC
[51320105014, 51321003, 51231008, 51501225]; CUPB [2462015YQ0602];
[U2014B0112]
FX The authors thank Dr. M.J. Zhuo, Dr. S.J. Zheng and Mr. L.P. You for the
insightful discussions. Thin film deposition of this work was supported
by the user proposal (U2014B0112) approved by the Center for Integrated
Nanotechnologies (CINT), a US Department of Energy, Office of Basic
Energy Sciences user facility at Los Alamos National Laboratory (LANL).
The TEM analysis portion of this work was supported by Electron
Microscopy Laboratory of Peking University. This work was supported by
ITER special funding with award number of 2015GB121004 from Ministry of
Science and Technology, and by Natural Science Foundation of China with
Award Number of 11375018 and 11528508. E.F. appreciates the support from
The Recruitment Program of Global Youth Experts in China, and the
Instrumental Analysis Fund of Peking University, and X.D. appreciates
the support of NSFC (51320105014, 51321003, and 51231008). K.Y.
appreciates the financial support of NSFC (51501225) and CUPB
(2462015YQ0602).
NR 50
TC 0
Z9 0
U1 18
U2 18
PU NATURE PUBLISHING GROUP
PI LONDON
PA MACMILLAN BUILDING, 4 CRINAN ST, LONDON N1 9XW, ENGLAND
SN 2045-2322
J9 SCI REP-UK
JI Sci Rep
PD OCT 4
PY 2016
VL 6
AR 33931
DI 10.1038/srep33931
PG 10
WC Multidisciplinary Sciences
SC Science & Technology - Other Topics
GA DX7VB
UT WOS:000384596400001
PM 27698458
ER
PT J
AU Brawand, NP
Voros, M
Govoni, M
Galli, G
AF Brawand, Nicholas P.
Voros, Marton
Govoni, Marco
Galli, Giulia
TI Generalization of Dielectric-Dependent Hybrid Functionals to Finite
Systems
SO PHYSICAL REVIEW X
LA English
DT Article
ID AB-INITIO CALCULATION; 1ST PRINCIPLES; ELECTRONIC EXCITATIONS; DENSITY
FUNCTIONALS; PERTURBATION-THEORY; QUANTUM-CHEMISTRY; GREENS-FUNCTION;
EXACT EXCHANGE; APPROXIMATION; NANOPARTICLES
AB The accurate prediction of electronic and optical properties of molecules and solids is a persistent challenge for methods based on density functional theory. We propose a generalization of dielectric-dependent hybrid functionals to finite systems where the definition of the mixing fraction of exact and semilocal exchange is physically motivated, nonempirical, and system dependent. The proposed functional yields ionization potentials, and fundamental and optical gaps of many, diverse molecular systems in excellent agreement with experiments, including organic and inorganic molecules and semiconducting nanocrystals. We further demonstrate that this hybrid functional gives the correct alignment between energy levels of the exemplary TTF-TCNQ donor-acceptor system.
C1 [Brawand, Nicholas P.; Voros, Marton; Govoni, Marco; Galli, Giulia] Univ Chicago, Inst Mol Engn, Chicago, IL 60637 USA.
[Voros, Marton; Govoni, Marco; Galli, Giulia] Argonne Natl Lab, Lemont, IL 60439 USA.
RP Galli, G (reprint author), Univ Chicago, Inst Mol Engn, Chicago, IL 60637 USA.; Galli, G (reprint author), Argonne Natl Lab, Lemont, IL 60439 USA.
EM gagalli@uchicago.edu
FU Center for Advanced Solar Photophysics, an Energy Frontier Research
Center - U.S. Department of Energy (DOE), Office of Science, Office of
Basic Energy Sciences; Laboratory Directed Research and Development
(LDRD) from Argonne National Laboratory [DE-AC02-06CH11357]; MICCoM,
Computational Materials Sciences Program - U.S. Department of Energy,
Office of Science, Basic Energy Sciences, Materials Sciences and
Engineering Division; Office of Science of the U.S. DOE
[DE-AC02-05CH11231]; DOE Office of Science User Facility
[DE-AC02-06CH11357]; U.S. Department of Energy National Nuclear Security
Administration [DE-AC52-06NA25396]
FX We are grateful for discussions with R. L. McAvoy, P. Scherpelz, A. P.
Gaiduk, J. Skone, and M. B. Goldey. Part of this project was supported
by the Center for Advanced Solar Photophysics, an Energy Frontier
Research Center funded by the U.S. Department of Energy (DOE), Office of
Science, Office of Basic Energy Sciences (N. B.) and by Laboratory
Directed Research and Development (LDRD) funding from Argonne National
Laboratory, provided by the Director, Office of Science, of the U.S.
Department of Energy under Contract No. DE-AC02-06CH11357 (M. V.). The
software developed in this project was supported by MICCoM (M. G. and G.
G.), as part of the Computational Materials Sciences Program funded by
the U.S. Department of Energy, Office of Science, Basic Energy Sciences,
Materials Sciences and Engineering Division. Computer time was provided
by the Innovative and Novel Computational Impact on Theory and
Experiment (INCITE) program; the National Energy Research Scientific
Computing Center, a DOE Office of Science User Facility supported by the
Office of Science of the U.S. DOE under Contract No. DE-AC02-05CH11231;
the Argonne Leadership Computing Facility, which is a DOE Office of
Science User Facility supported under Contract No. DE-AC02-06CH11357 and
the Los Alamos National Laboratory Institutional Computing Program,
which is supported by the U.S. Department of Energy National Nuclear
Security Administration under Contract No. DE-AC52-06NA25396.
NR 88
TC 3
Z9 3
U1 10
U2 10
PU AMER PHYSICAL SOC
PI COLLEGE PK
PA ONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA
SN 2160-3308
J9 PHYS REV X
JI Phys. Rev. X
PD OCT 4
PY 2016
VL 6
IS 4
AR 041002
DI 10.1103/PhysRevX.6.041002
PG 9
WC Physics, Multidisciplinary
SC Physics
GA DX8AV
UT WOS:000384611400001
ER
PT J
AU Khachatryan, V
Sirunyan, AM
Tumasyan, A
Adam, W
Asilar, E
Bergauer, T
Brandstetter, J
Brondolin, E
Dragicevic, M
Ero, J
Flechl, M
Friedl, M
Fruhwirth, R
Ghete, VM
Hormann, N
Hrubec, J
Jeitler, M
Konig, A
Kratschmer, I
Liko, D
Matsushita, T
Mikulec, I
Rabady, D
Rad, N
Rahbaran, B
Rohringer, H
Schieck, J
Strauss, J
Treberer-Treberspurg, W
Waltenberger, W
Wulz, CE
Mossolov, V
Shumeiko, N
Gonzalez, JS
Alderweireldt, S
Cornelis, T
De Wolf, EA
Janssen, X
Knutsson, A
Lauwers, J
De Klundert, MV
Van Haevermaet, H
Van Mechelen, P
Van Remortel, N
Van Spilbeeck, A
Abu Zeid, S
Blekman, F
D'Hondt, J
Daci, N
De Bruyn, I
Deroover, K
Heracleous, N
Lowette, S
Moortgat, S
Moreels, L
Olbrechts, A
Python, Q
Tavernier, S
Van Doninck, W
Van Mulders, P
Van Parijs, I
Brun, H
Caillol, C
Clerbaux, B
De Lentdecker, G
Delannoy, H
Fasanella, G
Favart, L
Goldouzian, R
Grebenyuk, A
Karapostoli, G
Lenzi, T
Leonard, A
Luetic, J
Maerschalk, T
Marinov, A
Randle-Conde, A
Seva, T
Velde, CV
Vanlaer, P
Yonamine, R
Zenoni, F
Zhang, F
Cimmino, A
Dobur, D
Fagot, A
Garcia, G
Gul, M
Mccartin, J
Poyraz, D
Salva, S
Schofbeck, R
Tytgat, M
Van Driessche, W
Yazgan, E
Zaganidis, N
Beluffi, C
Bondu, O
Brochet, S
Bruno, G
Caudron, A
Ceard, L
De Visscher, S
Delaere, C
Delcourt, M
Forthomme, L
Francois, B
Giammanco, A
Jafari, A
Jez, P
Komm, M
Lemaitre, V
Magitteri, A
Mertens, A
Musich, M
Nuttens, C
Piotrzkowski, K
Quertenmont, L
Selvaggi, M
Marono, MV
Wertz, S
Beliy, N
Alda, WL
Alves, FL
Alves, GA
Brito, L
Hamer, M
Hensel, C
Moraes, A
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CA CMS Collaboration
TI Search for new physics with the M-T2 variable in all-jets final states
produced in pp collisions at root s=13 Tev
SO JOURNAL OF HIGH ENERGY PHYSICS
LA English
DT Article
DE Hadron-Hadron scattering (experiments); Supersymmetry
ID HADRON COLLIDERS; SUPERGAUGE TRANSFORMATIONS; GLUINO PRODUCTION;
MEASURING MASSES; MISSING ENERGY; SQUARK; MODEL; EXTENSION; INVARIANT;
NEUTRINO
AB A search for new physics is performed using events that contain one or more jets, no isolated leptons, and a large transverse momentum imbalance, as measured through the M-T2 variable, which is an extension of the transverse mass in events with two invisible particles. The results are based on a sample of proton-proton collisions collected at a center-of-mass energy of 13 TeV with the CMS detector at the LHC, and that corresponds to an integrated luminosity of 2.3 fb(-1). The observed event yields in the data are consistent with predictions for the standard model backgrounds. The results are interpreted using simplified models of supersymmetry and are expressed in terms of limits on the masses of potential new colored particles. Assuming that the lightest neutralino is stable and has a mass less than about 500 GeV, gluino masses up to 1550-1750 GeV are excluded at 95% confidence level, depending on the gluino decay mechanism. For the scenario of direct production of squark-antisquark pairs, top squarks with masses up to 800 GeV are excluded, assuming a 100% branching fraction for the decay to a top quark and neutralino. Similarly, bottom squark masses are excluded up to 880 GeV, and masses of light-flavor squarks are excluded up to 600-1260 GeV, depending on the degree of degeneracy of the squark masses.
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[Buontempo, S.; Cavallo, N.; Di Guida, S.; Esposito, M.; Fabozzi, F.; Iorio, A. O. M.; Lanza, G.; Lista, L.; Meola, S.; Merola, M.; Paolucci, P.; Sciacca, C.] Ist Nazl Fis Nucl, Sez Napoli, Naples, Italy.
[Esposito, M.; Iorio, A. O. M.; Sciacca, C.] Univ Naples Federico II, Naples, Italy.
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[Di Guida, S.; Meola, S.] Univ G Marconi, Rome, Italy.
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[Braghieri, A.; Magnani, A.; Montagna, P.; Ratti, S. P.; Re, V.; Riccardi, C.; Salvini, P.; Vai, I.; Vitulo, P.] Ist Nazl Fis Nucl, Sez Pavia, Pavia, Italy.
[Magnani, A.; Montagna, P.; Ratti, S. P.; Riccardi, C.; Vai, I.; Vitulo, P.] Univ Pavia, Pavia, Italy.
[Solestizi, L. Alunni; Bilei, G. M.; Ciangottini, D.; Fano, L.; Lariccia, P.; Leonardi, R.; Mantovani, G.; Menichelli, M.; Saha, A.; Santocchia, A.] Ist Nazl Fis Nucl, Sez Perugia, Perugia, Italy.
[Solestizi, L. Alunni; Ciangottini, D.; Fano, L.; Lariccia, P.; Leonardi, R.; Mantovani, G.; Santocchia, A.] Univ Perugia, Perugia, Italy.
[Androsov, K.; Azzurri, P.; Bagliesi, G.; Bernardini, J.; Boccali, T.; Castaldi, R.; Ciocci, M. A.; Dell'Orso, R.; Donato, S.; Giassi, A.; Grippo, M. T.; Ligabue, F.; Lomtadze, T.; Martini, L.; Messineo, A.; Palla, F.; Rizzi, A.; Savoy-Navarro, A.; Spagnolo, P.; Tenchini, R.; Tonelli, G.; Venturi, A.; Verdini, P. G.] Ist Nazl Fis Nucl, Sez Pisa, Pisa, Italy.
[Martini, L.; Messineo, A.; Rizzi, A.; Tonelli, G.] Univ Pisa, Pisa, Italy.
[Donato, S.; Ligabue, F.] Scuola Normale Super Pisa, Pisa, Italy.
[Barone, L.; Cavallari, F.; Cipriani, M.; D'imperio, G.; Del Re, D.; Diemoz, M.; Gelli, S.; Jorda, C.; Longo, E.; Margaroli, F.; Meridiani, P.; Organtini, G.; Paramatti, R.; Preiato, F.; Rahatlou, S.; Rovelli, C.; Santanastasio, F.] Ist Nazl Fis Nucl, Sez Roma, Rome, Italy.
[Barone, L.; Cipriani, M.; D'imperio, G.; Del Re, D.; Gelli, S.; Longo, E.; Margaroli, F.; Organtini, G.; Preiato, F.; Rahatlou, S.; Santanastasio, F.] Univ Roma, Rome, Italy.
[Amapane, N.; Arcidiacono, R.; Argiro, S.; Arneodo, M.; Bartosik, N.; Bellan, R.; Biino, C.; Cartiglia, N.; Costa, M.; Covarelli, R.; Degano, A.; Demaria, N.; Finco, L.; Kiani, B.; Mariotti, C.; Maselli, S.; Migliore, E.; Monaco, V.; Monteil, E.; Obertino, M. M.; Pacher, L.; Pastrone, N.; Pelliccioni, M.; Angioni, G. L. Pinna; Ravera, F.; Romero, A.; Ruspa, M.; Sacchi, R.; Shchelina, K.; Sola, V.; Solano, A.; Staiano, A.; Traczyk, P.] Ist Nazl Fis Nucl, Sez Torino, Turin, Italy.
[Amapane, N.; Argiro, S.; Bellan, R.; Costa, M.; Covarelli, R.; Degano, A.; Finco, L.; Kiani, B.; Migliore, E.; Monaco, V.; Monteil, E.; Obertino, M. M.; Pacher, L.; Angioni, G. L. Pinna; Ravera, F.; Romero, A.; Sacchi, R.; Shchelina, K.; Solano, A.; Traczyk, P.] Univ Torino, Turin, Italy.
[Arcidiacono, R.; Arneodo, M.; Ruspa, M.] Univ Piemonte Orientale, Novara, Italy.
[Belforte, S.; Candelise, V.; Casarsa, M.; Cossutti, F.; Della Ricca, G.; La Licata, C.; Schizzi, A.; Zanetti, A.] Ist Nazl Fis Nucl, Sez Trieste, Trieste, Italy.
[Candelise, V.; Della Ricca, G.; La Licata, C.; Schizzi, A.] Univ Trieste, Trieste, Italy.
[Kim, D. H.; Kim, G. N.; Kim, M. S.; Lee, S.; Lee, S. W.; Oh, Y. D.; Sekmen, S.; Son, D. C.; Yang, Y. C.] Kyungpook Natl Univ, Daegu, South Korea.
[Kim, H.; Lee, A.] Chonbuk Natl Univ, Jeonju, South Korea.
[Cifuentes, J. A. Brochero; Kim, T. J.] Hanyang Univ, Seoul, South Korea.
[Cho, S.; Choi, S.; Go, Y.; Gyun, D.; Ha, S.; Hong, B.; Jo, Y.; Kim, Y.; Lee, B.; Lee, K.; Lee, K. S.; Lee, S.; Lim, J.; Park, S. K.; Roh, Y.] Korea Univ, Seoul, South Korea.
[Almond, J.; Kim, J.; Oh, S. B.; Seo, S. H.; Yang, U. K.; Yoo, H. D.; Yu, G. B.] Seoul Natl Univ, Seoul, South Korea.
[Choi, M.; Kim, J. H.; Lee, J. S. H.; Park, I. C.; Ryu, G.; Ryu, M. S.] Univ Seoul, Seoul, South Korea.
[Choi, Y.; Goh, J.; Kim, D.; Kwon, E.; Lee, J.; Yu, I.] Sungkyunkwan Univ, Suwon, South Korea.
[Dudenas, V.; Juodagalvis, A.; Vaitkus, J.] Vilnius Univ, Vilnius, Lithuania.
[Ahmed, I.; Ibrahim, Z. A.; Komaragiri, J. R.; Ali, M. A. B. Md; Idris, F. Mohamad; Abdullah, W. A. T. Wan; Yusli, M. N.; Zolkapli, Z.] Univ Malaya, Natl Ctr Particle Phys, Kuala Lumpur, Malaysia.
[Casimiro Linares, E.; Castilla-Valdez, H.; De La Cruz-Burelo, E.; Heredia-De La Cruz, I.; Hernandez-Almada, A.; Lopez-Fernandez, R.; Mejia Guisao, J.; Sanchez-Hernandez, A.] IPN, Ctr Invest & Estudios Avanzados, Mexico City, DF, Mexico.
[Carrillo Moreno, S.; Vazquez Valencia, F.] Univ Iberoamer, Mexico City, DF, Mexico.
[Pedraza, I.; Salazar Ibarguen, H. A.; Uribe Estrada, C.] Benemerita Univ Autonoma Puebla, Puebla, Mexico.
[Morelos Pineda, A.] Univ Autonoma San Luis Potosi, San Luis Potosi, Mexico.
[Krofcheck, D.] Univ Auckland, Auckland, New Zealand.
[Butler, P. H.] Univ Canterbury, Christchurch, New Zealand.
[Ahmad, A.; Ahmad, M.; Hassan, Q.; Hoorani, H. R.; Khan, W. A.; Khurshid, T.; Shoaib, M.; Waqas, M.] Quaid I Azam Univ, Natl Ctr Phys, Islamabad, Pakistan.
[Bialkowska, H.; Bluj, M.; Boimska, B.; Frueboes, T.; Gorski, M.; Kazana, M.; Nawrocki, K.; Romanowska-Rybinska, K.; Szleper, M.; Zalewski, P.] Natl Ctr Nucl Res, Otwock, Poland.
[Bunkowski, K.; Byszuk, A.; Doroba, K.; Kalinowski, A.; Konecki, M.; Krolikowski, J.; Misiura, M.; Olszewski, M.; Walczak, M.] Univ Warsaw, Fac Phys, Inst Expt Phys, Warsaw, Poland.
[Bargassa, P.; Beirao Da Cruz E Silva, C.; Di Francesco, A.; Faccioli, P.; Ferreira Parracho, P. G.; Gallinaro, M.; Hollar, J.; Leonardo, N.; Lloret Iglesias, L.; Nemallapudi, M. V.; Rodrigues Antunes, J.; Seixas, J.; Toldaiev, O.; Vadruccio, D.; Varela, J.; Vischia, P.] Lab Instrumentacao & Fis Expt Particulas, Lisbon, Portugal.
[Khvedelidze, A.; Tsamalaidze, Z.; Bunin, P.; Gavrilenko, M.; Gorbunov, I.; Karjavin, V.; Lanev, A.; Malakhov, A.; Matveev, V.; Moisenz, P.; Palichik, V.; Perelygin, V.; Savina, M.; Shmatov, S.; Shulha, S.; Skatchkov, N.; Smirnov, V.; Voytishin, N.; Yuldashev, B. S.; Zarubin, A.] Joint Inst Nucl Res, Dubna, Russia.
[Chtchipounov, L.; Golovtsov, V.; Ivanov, Y.; Kim, V.; Kuznetsova, E.; Murzin, V.; Oreshkin, V.; Sulimov, V.; Vorobyev, A.] Petersburg Nucl Phys Inst, Gatchina, St Petersburg, Russia.
[Andreev, Yu.; Dermenev, A.; Gninenko, S.; Golubev, N.; Karneyeu, A.; Kirsanov, M.; Krasnikov, N.; Pashenkov, A.; Tlisov, D.; Toropin, A.] Inst Nucl Res, Moscow, Russia.
[Epshteyn, V.; Gavrilov, V.; Lychkovskaya, N.; Popov, V.; Pozdnyakov, I.; Safronov, G.; Spiridonov, A.; Toms, M.; Vlasov, E.; Zhokin, A.] Inst Theoret & Expt Phys, Moscow, Russia.
[Chadeeva, M.; Danilov, M.; Tarkovskii, E.] Natl Res Nucl Univ, Moscow Engn Phys Inst MEPhI, Moscow, Russia.
[Andreev, V.; Azarkin, M.; Dremin, I.; Kirakosyan, M.; Leonidov, A.; Rusakov, S. V.; Terkulov, A.] PN Lebedev Phys Inst, Moscow, Russia.
[Zhukov, V.; Katkov, I.; Baskakov, A.; Belyaev, A.; Boos, E.; Dubinin, M.; Dudko, L.; Ershov, A.; Gribushin, A.; Klyukhin, V.; Kodolova, O.; Lokhtin, I.; Miagkov, I.; Obraztsov, S.; Petrushanko, S.; Savrin, V.; Snigirev, A.] Lomonosov Moscow State Univ, Skobeltsyn Inst Nucl Phys, Moscow, Russia.
[Azhgirey, I.; Bayshev, I.; Bitioukov, S.; Elumakhov, D.; Kachanov, V.; Kalinin, A.; Konstantinov, D.; Krychkine, V.; Petrov, V.; Ryutin, R.; Sobol, A.; Troshin, S.; Tyurin, N.; Uzunian, A.; Volkov, A.] State Res Ctr Russian Federat, Inst High Energy Phys, Protvino, Russia.
[Adzic, P.; Cirkovic, P.; Devetak, D.; Milosevic, J.; Rekovic, V.] Univ Belgrade, Fac Phys, Belgrade, Serbia.
[Adzic, P.; Cirkovic, P.; Devetak, D.; Milosevic, J.; Rekovic, V.] Vinca Inst Nucl Sci, Belgrade, Serbia.
[Alcaraz Maestre, J.; Calvo, E.; Cerrada, M.; Chamizo Llatas, M.; Colino, N.; De La Cruz, B.; Delgado Peris, A.; Escalante Del Valle, A.; Fernandez Bedoya, C.; Fernandez Ramos, J. P.; Flix, J.; Fouz, M. C.; Garcia-Abia, P.; Gonzalez Lopez, O.; Goy Lopez, S.; Hernandez, J. M.; Josa, M. I.; Navarro De Martino, E.; Perez-Calero Yzquierdo, A.; Puerta Pelayo, J.; Quintario Olmeda, A.; Redondo, I.; Romero, L.; Soares, M. S.] Ctr Invest Energet Medioambientales & Tecnol CIEM, Madrid, Spain.
[de Troconiz, J. F.; Missiroli, M.; Moran, D.] Univ Autonoma Madrid, Madrid, Spain.
[Cuevas, J.; Fernandez Menendez, J.; Gonzalez Caballero, I.; Palencia Cortezon, E.; Sanchez Cruz, S.; Vizan Garcia, J. M.] Univ Oviedo, Oviedo, Spain.
[Cabrillo, I. J.; Calderon, A.; Castineiras De Saa, J. R.; Curras, E.; Fernandez, M.; Garcia-Ferrero, J.; Gomez, G.; Lopez Virto, A.; Marco, J.; Martinez Rivero, C.; Matorras, F.; Piedra Gomez, J.; Rodrigo, T.; Ruiz-Jimeno, A.; Scodellaro, L.; Trevisani, N.; Vila, I.; Vilar Cortabitarte, R.] Univ Cantabria, CSIC, Inst Fis Cantabria IFCA, Santander, Spain.
[Stahl, A.; Pantaleo, F.; Hartmann, F.; Kornmayer, A.; Mohanty, A. K.; Silvestris, L.; Viliani, L.; Primavera, F.; Manzoni, R. A.; Di Guida, S.; Meola, S.; Paolucci, P.; Azzi, P.; Pazzini, J.; Azzurri, P.; D'imperio, G.; Del Re, D.; Arcidiacono, R.; Abbaneo, D.; Auffray, E.; Auzinger, G.; Bachtis, M.; Baillon, P.; Ball, A. H.; Barney, D.; Bloch, P.; Bocci, A.; Bonato, A.; Botta, C.; Camporesi, T.; Castello, R.; Cepeda, M.; Cerminara, G.; D'Alfonso, M.; d'Enterria, D.; Dabrowski, A.; Daponte, V.; David, A.; De Gruttola, M.; De Guio, F.; De Roeck, A.; Di Marco, E.; Dobson, M.; Dordevic, M.; Dorney, B.; du Pree, T.; Duggan, D.; Duenser, M.; Dupont, N.; Elliott-Peisert, A.; Fartoukh, S.; Franzoni, G.; Fulcher, J.; Funk, W.; Gigi, D.; Gill, K.; Girone, M.; Glege, F.; Gundacker, S.; Guthoff, M.; Hammer, J.; Harris, P.; Hegeman, J.; Innocente, V.; Janot, P.; Kirschenmann, H.; Knuenz, V.; Kortelainen, M. J.; Kousouris, K.; Krammer, M.; Lecoq, P.; Lourenco, C.; Lucchini, M. T.; Magini, N.; Malgeri, L.; Mannelli, M.; Martelli, A.; Meijers, F.; Mersi, S.; Meschi, E.; Moortgat, F.; Morovic, S.; Mulders, M.; Neugebauer, H.; Orfanelli, S.; Orsini, L.; Pape, L.; Perez, E.; Peruzzi, M.; Petrilli, A.; Petrucciani, G.; Er, A. Pfei Ff; Pierini, M.; Racz, A.; Reis, T.; Rolandi, G.; Rovere, M.; Ruan, M.; Sakulin, H.; Sauvan, J. B.; Schaefer, C.; Schwick, C.; Seidel, M.; Sharma, A.; Silva, P.; Simon, M.; Sphicas, P.; Steggemann, J.; Stoye, M.; Takahashi, Y.; Treille, D.; Triossi, A.; Tsirou, A.; Veckalns, V.; Veres, G. I.; Wardle, N.; Zagozdzinska, A.; Zeuner, W. D.; Virdee, T.] CERN, European Org Nucl Res, CH-1211 Geneva, Switzerland.
[Bertl, W.; Deiters, K.; Erdmann, W.; Horisberger, R.; Ingram, Q.; Kaestli, H. C.; Kotlinski, D.; Langenegger, U.; Rohe, T.] Paul Scherrer Inst, Villigen, Switzerland.
[Bachmair, F.; Baeni, L.; Bianchini, L.; Casal, B.; Dissertori, G.; Dittmar, M.; Donega, M.; Eller, P.; Grab, C.; Heidegger, C.; Hits, D.; Hoss, J.; Kasieczka, G.; Lecomte, P.; Lustermann, W.; Mangano, B.; Marionneau, M.; del Arbol, P. Martinez Ruiz; Masciovecchio, M.; Meinhard, M. T.; Meister, D.; Micheli, F.; Musella, P.; Nessi-Tedaldi, F.; Pandolfi, F.; Pata, J.; Pauss, F.; Perrin, G.; Perrozzi, L.; Quittnat, M.; Rossini, M.; Schoenenberger, M.; Starodumov, A.; Takahashi, M.; Tavolaro, V. R.; Theofilatos, K.; Wallny, R.] Swiss Fed Inst Technol, Inst Particle Phys, Zurich, Switzerland.
[Aarrestad, T. K.; Amsler, C.; Caminada, L.; Canelli, M. F.; Chiochia, V.; De Cosa, A.; Galloni, C.; Hinzmann, A.; Hreus, T.; Kilminster, B.; Lange, C.; Ngadiuba, J.; Pinna, D.; Rauco, G.; Robmann, P.; Salerno, D.; Yang, Y.] Univ Zurich, Zurich, Switzerland.
[Doan, T. H.; Jain, Sh.; Khurana, R.; Konyushikhin, M.; Kuo, C. M.; Lin, W.; Lu, Y. J.; Pozdnyakov, A.; Yu, S. S.] Natl Cent Univ, Chungli, Taiwan.
[Kumar, Arun; Chang, P.; Chang, Y. H.; Chang, Y. W.; Chao, Y.; Chen, K. F.; Chen, P. H.; Dietz, C.; Fiori, F.; Hou, W. -S.; Hsiung, Y.; Liu, Y. F.; Lu, R. -S.; Moya, M. Minano; Paganis, E.; Psallidas, A.; Tsai, J. F.; Tzeng, Y. M.] Natl Taiwan Univ, Taipei, Taiwan.
[Asavapibhop, B.; Singh, G.; Srimanobhas, N.; Suwonjandee, N.] Chulalongkorn Univ, Fac Sci, Dept Phys, Bangkok, Thailand.
[Adiguzel, A.; Cerci, S.; Damarseckin, S.; Demiroglu, Z. S.; Dozen, C.; Dumanoglu, I.; Girgis, S.; Gokbulut, G.; Guler, Y.; Gurpinar, E.; Hos, I.; Kangal, E. E.; Topaksu, A. Kayis; Onengut, G.; Ozdemir, K.; Cerci, D. Sunar; Tali, B.; Zorbilmez, C.] Cukurova Univ, Adana, Turkey.
[Bilin, B.; Bilmis, S.; Isildak, B.; Karapinar, G.; Yalvac, M.; Zeyrek, M.] Middle East Tech Univ, Dept Phys, Ankara, Turkey.
[Gulmez, E.; Kaya, M.; Kaya, O.; Yetkin, E. A.; Yetkin, T.] Bogazici Univ, Istanbul, Turkey.
[Cakir, A.; Cankocak, K.; Sen, S.; Vardarli, F. I.] Istanbul Tech Univ, Istanbul, Turkey.
[Grynyov, B.] Natl Acad Sci Ukraine, Inst Scintillat Mat, Kharkov, Ukraine.
[Levchuk, L.; Sorokin, P.] Natl Sci Ctr Kharkov Inst Phys & Technol, Kharkov, Ukraine.
[Aggleton, R.; Ball, F.; Beck, L.; Brooke, J. J.; Burns, D.; Clement, E.; Cussans, D.; Flacher, H.; Goldstein, J.; Grimes, M.; Heath, G. P.; Heath, H. F.; Jacob, J.; Kreczko, L.; Lucas, C.; Meng, Z.; Newbold, D. M.; Paramesvaran, S.; Poll, A.; Sakuma, T.; El Nasr-Storey, S. Seif; Senkin, S.; Smith, D.; Smith, V. J.] Univ Bristol, Bristol, Avon, England.
[Bell, K. W.; Belyaev, A.; Brew, C.; Brown, R. M.; Calligaris, L.; Cieri, D.; Cockerill, D. J. A.; Coughlan, J. A.; Harder, K.; Harper, S.; Olaiya, E.; Petyt, D.; Shepherd-Themistocleous, C. H.; Thea, A.; Tomalin, I. R.; Williams, T.] Rutherford Appleton Lab, Didcot, Oxon, England.
[Baber, M.; Bainbridge, R.; Buchmuller, O.; Bundock, A.; Burton, D.; Casasso, S.; Citron, M.; Colling, D.; Corpe, L.; Dauncey, P.; Davies, G.; De Wit, A.; Della Negra, M.; Dunne, P.; Elwood, A.; Futyan, D.; Haddad, Y.; Hall, G.; Iles, G.; Lane, R.; Laner, C.; Lucas, R.; Lyons, L.; Magnan, A. -M.; Malik, S.; Mastrolorenzo, L.; Nash, J.; Nikitenko, A.; Pela, J.; Penning, B.; Pesaresi, M.; Raymond, D. M.; Richards, A.; Rose, A.; Seez, C.; Tapper, A.; Uchida, K.; Acosta, M. Vazquez; Virdee, T.] Imperial Coll, London, England.
[Cole, J. E.; Hobson, P. R.; Khan, A.; Kyberd, P.; Leslie, D.; Reid, I. D.; Symonds, P.; Teodorescu, L.; Turner, M.] Brunel Univ, Uxbridge, Middx, England.
[Borzou, A.; Call, K.; Dittmann, J.; Hatakeyama, K.; Liu, H.; Pastika, N.] Baylor Univ, Waco, TX 76798 USA.
[Charaf, O.; Cooper, S. I.; Henderson, C.; Rumerio, P.] Univ Alabama, Tuscaloosa, AL USA.
[Aleksandrov, A.; Arcaro, D.; Avetisyan, A.; Bose, T.; Gastler, D.; Rankin, D.; Richardson, C.; Rohlf, J.; Sulak, L.; Zou, D.] Boston Univ, Boston, MA 02215 USA.
[Benelli, G.; Berry, E.; Cutts, D.; Ferapontov, A.; Garabedian, A.; Hakala, J.; Heintz, U.; Jesus, O.; Laird, E.; Landsberg, G.; Mao, Z.; Narain, M.; Piperov, S.; Sagir, S.; Spencer, E.; Syarif, R.] Brown Univ, Providence, RI 02912 USA.
[Breedon, R.; Breto, G.; Burns, D.; Sanchez, M. Calderon De La Barca; Chauhan, S.; Chertok, M.; Conway, J.; Conway, R.; Cox, P. T.; Erbacher, R.; Flores, C.; Funk, G.; Gardner, M.; Ko, W.; Lander, R.; Mclean, C.; Mulhearn, M.; Pellett, D.; Pilot, J.; Ricci-Tam, F.; Shalhout, S.; Smith, J.; Squires, M.; Stolp, D.; Tripathi, M.; Wilbur, S.; Yohay, R.] Univ Calif Davis, Davis, CA 95616 USA.
[Cousins, R.; Everaerts, P.; Florent, A.; Hauser, J.; Ignatenko, M.; Saltzberg, D.; Takasugi, E.; Valuev, V.; Weber, M.] Univ Calif Los Angeles, Los Angeles, CA USA.
[Burt, K.; Clare, R.; Ellison, J.; Gary, J. W.; Hanson, G.; Heilman, J.; Jandir, P.; Kennedy, E.; Lacroix, F.; Long, O. R.; Malberti, M.; Negrete, M. Olmedo; Paneva, M. I.; Shrinivas, A.; Wei, H.; Wimpenny, S.; Yates, B. R.] Univ Calif Riverside, Riverside, CA 92521 USA.
[Branson, J. G.; Cerati, G. B.; Cittolin, S.; D'Agnolo, R. T.; Derdzinski, M.; Gerosa, R.; Holzner, A.; Kelley, R.; Klein, D.; Letts, J.; Macneill, I.; Olivito, D.; Padhi, S.; Pieri, M.; Sani, M.; Sharma, V.; Simon, S.; Tadel, M.; Vartak, A.; Wasserbaech, S.; Welke, C.; Wood, J.; Wuerthwein, F.; Yagil, A.; Della Porta, G. Zevi] Univ Calif San Diego, La Jolla, CA 92093 USA.
[Bhandari, R.; Bradmiller-Feld, J.; Campagnari, C.; Dishaw, A.; Dutta, V.; Flowers, K.; Sevilla, M. Franco; Ert, P. Ge Ff; George, C.; Golf, F.; Gouskos, L.; Gran, J.; Heller, R.; Incandela, J.; Mccoll, N.; Mullin, S. D.; Ovcharova, A.; Richman, J.; Stuart, D.; Suarez, I.; West, C.; Yoo, J.] Univ Calif Santa Barbara, Santa Barbara, CA 93106 USA.
[Anderson, D.; Apresyan, A.; Bendavid, J.; Bornheim, A.; Bunn, J.; Chen, Y.; Duarte, J.; Mott, A.; Newman, H. B.; Pena, C.; Spiropulu, M.; Vlimant, J. R.; Xie, S.; Zhu, R. Y.] CALTECH, Pasadena, CA 91125 USA.
[Andrews, M. B.; Azzolini, V.; Calamba, A.; Carlson, B.; Ferguson, T.; Paulini, M.; Russ, J.; Sun, M.; Vogel, H.; Vorobiev, I.] Carnegie Mellon Univ, Pittsburgh, PA 15213 USA.
[Cumalat, J. P.; Ford, W. T.; Jensen, F.; Johnson, A.; Krohn, M.; Mulholland, T.; Stenson, K.; Wagner, S. R.] Univ Colorado Boulder, Boulder, CO USA.
[Alexander, J.; Chaves, J.; Chu, J.; Dittmer, S.; Mirman, N.; Kaufman, G. Nicolas; Patterson, J. R.; Rinkevicius, A.; Ryd, A.; Skinnari, L.; Sun, W.; Tan, S. M.; Tao, Z.; Thom, J.; Tucker, J.; Wittich, P.] Cornell Univ, Ithaca, NY USA.
[Winn, D.] Fairfield Univ, Fairfield, CT 06430 USA.
[Abdullin, S.; Albrow, M.; Apollinari, G.; Banerjee, S.; Bauerdick, L. A. T.; Beretvas, A.; Berryhill, J.; Bhat, P. C.; Bolla, G.; Burkett, K.; Butler, J. N.; Cheung, H. W. K.; Chlebana, F.; Cihangir, S.; Cremonesi, M.; Elvira, V. D.; Fisk, I.; Freeman, J.; Gottschalk, E.; Gray, L.; Green, D.; Gruenendahl, S.; Gutsche, O.; Hare, D.; Harris, R. M.; Hasegawa, S.; Hirschauer, J.; Hu, Z.; Jayatilaka, B.; Jindariani, S.; Johnson, M.; Joshi, U.; Klima, B.; Kreis, B.; Lammel, S.; Linacre, J.; Lincoln, D.; Lipton, R.; Liu, T.; De Sa, R. Lopes; Lykken, J.; Marraffino, J. M.; Maruyama, S.; Mason, D.; McBride, P.; Merkel, P.; Mrenna, S.; Nahn, S.; Newman-Holmes, C.; O'Dell, V.; Pedro, K.; Prokofyev, O.; Rakness, G.; Ristori, L.; Sexton-Kennedy, E.; Soha, A.; Spalding, W. J.; Spiegel, L.; Stoynev, S.; Strobbe, N.; Taylor, L.; Tkaczyk, S.; Tran, N. V.; Uplegger, L.; Vaandering, E. W.; Vernieri, C.; Verzocchi, M.; Vidal, R.; Wang, M.; Weber, H. A.; Whitbeck, A.] Fermilab Natl Accelerator Lab, POB 500, Batavia, IL 60510 USA.
[Acosta, D.; Avery, P.; Bortignon, P.; Bourilkov, D.; Brinkerhoff, A.; Carnes, A.; Carver, M.; Curry, D.; Das, S.; Field, R. D.; Furic, I. K.; Konigsberg, J.; Korytov, A.; Ma, P.; Matchev, K.; Mei, H.; Milenovic, P.; Mitselmakher, G.; Rank, D.; Shchutska, L.; Sperka, D.; Thomas, L.; Wang, J.; Wang, S.; Yelton, J.] Univ Florida, Gainesville, FL USA.
[Linn, S.; Markowitz, P.; Martinez, G.; Rodriguez, J. L.] Florida Int Univ, Miami, FL 33199 USA.
[Ackert, A.; Adams, J. R.; Adams, T.; Askew, A.; Bein, S.; Diamond, B.; Hagopian, S.; Hagopian, V.; Johnson, K. F.; Khatiwada, A.; Prosper, H.; Santra, A.; Weinberg, M.] Florida State Univ, Tallahassee, FL 32306 USA.
[Baarmand, M. M.; Bhopatkar, V.; Colafranceschi, S.; Hohlmann, M.; Kalakhety, H.; Noonan, D.; Roy, T.; Yumiceva, F.] Florida Inst Technol, Melbourne, FL 32901 USA.
[Adams, M. R.; Apanasevich, L.; Berry, D.; Betts, R. R.; Bucinskaite, I.; Cavanaugh, R.; Evdokimov, O.; Gauthier, L.; Gerber, C. E.; Hofman, D. J.; Kurt, P.; O'Brien, C.; Gonzalez, I. D. Sandoval; Turner, P.; Varelas, N.; Wu, Z.; Zakaria, M.; Zhang, J.] Univ Illinois, Chicago, IL USA.
[Bilki, B.; Clarida, W.; Dilsiz, K.; Durgut, S.; Gandrajula, R. P.; Haytmyradov, M.; Khristenko, V.; Merlo, J. -P.; Mermerkaya, H.; Mestvirishvili, A.; Moeller, A.; Nachtman, J.; Ogul, H.; Onel, Y.; Ozok, F.; Penzo, A.; Snyder, C.; Tiras, E.; Wetzel, J.; Yi, K.] Univ Iowa, Iowa City, IA USA.
[Anderson, I.; Blumenfeld, B.; Cocoros, A.; Eminizer, N.; Fehling, D.; Feng, L.; Gritsan, A. V.; Maksimovic, P.; Osherson, M.; Roskes, J.; Sarica, U.; Swartz, M.; Xiao, M.; Xin, Y.; You, C.] Johns Hopkins Univ, Baltimore, MD USA.
[Al-Bataineh, A.; Baringer, P.; Bean, A.; Bowen, J.; Bruner, C.; Castle, J.; Kenny, R. P., III; Kropivnitskaya, A.; Majumder, D.; Mcbrayer, W.; Murray, M.; Sanders, S.; Stringer, R.; Takaki, J. D. Tapia; Wang, Q.] Univ Kansas, Lawrence, KS 66045 USA.
[Ivanov, A.; Kaadze, K.; Khalil, S.; Makouski, M.; Maravin, Y.; Mohammadi, A.; Saini, L. K.; Skhirtladze, N.; Toda, S.] Kansas State Univ, Manhattan, KS 66506 USA.
[Lange, D.; Rebassoo, F.; Wright, D.] Lawrence Livermore Natl Lab, Livermore, CA USA.
[Anelli, C.; Baden, A.; Baron, O.; Belloni, A.; Calvert, B.; Eno, S. C.; Ferraioli, C.; Gomez, J. A.; Hadley, N. J.; Jabeen, S.; Kellogg, R. G.; Kolberg, T.; Kunkle, J.; Lu, Y.; Mignerey, A. C.; Shin, Y. H.; Skuja, A.; Tonjes, M. B.; Tonwar, S. C.] Univ Maryland, College Pk, MD 20742 USA.
[Apyan, A.; Barbieri, R.; Baty, A.; Bi, R.; Bierwagen, K.; Brandt, S.; Busza, W.; Cali, I. A.; Demiragli, Z.; Di Matteo, L.; Ceballos, G. Gomez; Goncharov, M.; Gulhan, D.; Hsu, D.; Iiyama, Y.; Innocenti, G. M.; Klute, M.; Kovalskyi, D.; Krajczar, K.; Lai, Y. S.; Lee, Y. -J.; Levin, A.; Luckey, P. D.; Marini, A. C.; Mcginn, C.; Mironov, C.; Narayanan, S.; Niu, X.; Paus, C.; Roland, C.; Roland, G.; Salfeld-Nebgen, J.; Stephans, G. S. F.; Sumorok, K.; Tatar, K.; Varma, M.; Velicanu, D.; Veverka, J.; Wang, J.; Wang, T. W.; Wyslouch, B.; Yang, M.; Zhukova, V.] MIT, Cambridge, MA 02139 USA.
[Benvenuti, A. C.; Chatterjee, R. M.; Dahmes, B.; Evans, A.; Finkel, A.; Gude, A.; Hansen, P.; Kalafut, S.; Kao, S. C.; Klapoetke, K.; Kubota, Y.; Lesko, Z.; Mans, J.; Nourbakhsh, S.; Ruckstuhl, N.; Rusack, R.; Tambe, N.; Turkewitz, J.] Univ Minnesota, Minneapolis, MN USA.
[Acosta, J. G.; Oliveros, S.] Univ Mississippi, Oxford, MS USA.
[Avdeeva, E.; Bartek, R.; Bloom, K.; Bose, S.; Claes, D. R.; Dominguez, A.; Fangmeier, C.; Suarez, R. Gonzalez; Kamalieddin, R.; Knowlton, D.; Kravchenko, I.; Meier, F.; Monroy, J.; Siado, J. E.; Snow, G. R.; Stieger, B.] Univ Nebraska Lincoln, Lincoln, NE USA.
[Alyari, M.; Dolen, J.; George, J.; Godshalk, A.; Harrington, C.; Iashvili, I.; Kaisen, J.; Kharchilava, A.; Kumar, A.; Parker, A.; Rappoccio, S.; Roozbahani, B.] SUNY Buffalo, Buffalo, NY USA.
[Alverson, G.; Barberis, E.; Baumgartel, D.; Chasco, M.; Hortiangtham, A.; Massironi, A.; Morse, D. M.; Nash, D.; Orimoto, T.; De Lima, R. Teixeira; Trocino, D.; Wang, R. -J.] Northeastern Univ, Boston, MA 02115 USA.
[Bhattacharya, S.; Hahn, K. A.; Kubik, A.; Low, J. F.; Mucia, N.; Odell, N.; Pollack, B.; Schmitt, M. H.; Sung, K.; Trovato, M.; Velasco, M.] Northwestern Univ, Evanston, IL USA.
[Dev, N.; Hildreth, M.; Anampa, K. Hurtado; Jessop, C.; Karmgard, D. J.; Kellams, N.; Lannon, K.; Marinelli, N.; Meng, F.; Mueller, C.; Musienko, Y.; Planer, M.; Reinsvold, A.; Ruchti, R.; Rupprecht, N.; Smith, G.; Taroni, S.; Valls, N.; Wayne, M.; Wolf, M.; Woodard, A.] Univ Notre Dame, Notre Dame, IN 46556 USA.
[Alimena, J.; Antonelli, L.; Brinson, J.; Bylsma, B.; Durkin, L. S.; Flowers, S.; Francis, B.; Hart, A.; Hill, C.; Hughes, R.; Ji, W.; Liu, B.; Luo, W.; Puigh, D.; Rodenburg, M.; Winer, B. L.; Wulsin, H. W.] Ohio State Univ, Columbus, OH 43210 USA.
[Cooperstein, S.; Driga, O.; Elmer, P.; Hardenbrook, J.; Hebda, P.; Luo, J.; Marlow, D.; Medvedeva, T.; Mooney, M.; Olsen, J.; Palmer, C.; Piroue, P.; Stickland, D.; Tully, C.; Zuranski, A.] Princeton Univ, Princeton, NJ 08544 USA.
[Malik, S.] Univ Puerto Rico, Mayaguez, PR USA.
[Barker, A.; Barnes, V. E.; Benedetti, D.; Folgueras, S.; Gutay, L.; Jha, M. K.; Jones, M.; Jung, A. W.; Jung, K.; Miller, D. H.; Neumeister, N.; Radburn-Smith, B. C.; Shi, X.; Sun, J.; Svyatkovskiy, A.; Wang, F.; Xie, W.; Xu, L.] Purdue Univ, W Lafayette, IN 47907 USA.
[Parashar, N.; Stupak, J.] Purdue Univ Calumet, Hammond, LA USA.
[Adair, A.; Akgun, B.; Chen, Z.; Ecklund, K. M.; Geurts, F. J. M.; Guilbaud, M.; Li, W.; Michlin, B.; Northup, M.; Padley, B. P.; Redjimi, R.; Roberts, J.; Rorie, J.; Tu, Z.; Zabel, J.] Rice Univ, Houston, TX USA.
[Betchart, B.; Bodek, A.; de Barbaro, P.; Demina, R.; Duh, Y. t.; Ferbel, T.; Galanti, M.; Garcia-Bellido, A.; Han, J.; Hindrichs, O.; Khukhunaishvili, A.; Lo, K. H.; Tan, P.; Verzetti, M.] Univ Rochester, Rochester, NY 14627 USA.
[Chou, J. P.; Contreras-Campana, E.; Gershtein, Y.; Espinosa, T. A. Gomez; Halkiadakis, E.; Heindl, M.; Hidas, D.; Hughes, E.; Kaplan, S.; Elayavalli, R. Kunnawalkam; Kyriacou, S.; Lath, A.; Nash, K.; Saka, H.; Salur, S.; Schnetzer, S.; Sheffield, D.; Somalwar, S.; Stone, R.; Thomas, S.; Thomassen, P.; Walker, M.] Rutgers State Univ, Piscataway, NJ USA.
[Foerster, M.; Heideman, J.; Riley, G.; Rose, K.; Spanier, S.; Thapa, K.] Univ Tennessee, Knoxville, TN USA.
[Bouhali, O.; Hernandez, A. Castaneda; Celik, A.; Dalchenko, M.; De Mattia, M.; Delgado, A.; Dildick, S.; Eusebi, R.; Gilmore, J.; Huang, T.; Juska, E.; Kamon, T.; Krutelyov, V.; Mueller, R.; Pakhotin, Y.; Patel, R.; Perloff, A.; Pernie, L.; Rathjens, D.; Rose, A.; Safonov, A.; Tatarinov, A.; Ulmer, K. A.] Texas A&M Univ, College Stn, TX USA.
[Akchurin, N.; Cowden, C.; Damgov, J.; Dragoiu, C.; Dudero, P. R.; Faulkner, J.; Kunori, S.; Lamichhane, K.; Lee, S. W.; Libeiro, T.; Undleeb, S.; Volobouev, I.; Wang, Z.] Texas Tech Univ, Lubbock, TX 79409 USA.
[Delannoy, A. G.; Greene, S.; Gurrola, A.; Janjam, R.; Johns, W.; Maguire, C.; Melo, A.; Ni, H.; Sheldon, P.; Tuo, S.; Velkovska, J.; Xu, Q.] Vanderbilt Univ, 221 Kirkland Hall, Nashville, TN 37235 USA.
[Arenton, M. W.; Barria, P.; Cox, B.; Goodell, J.; Hirosky, R.; Ledovskoy, A.; Li, H.; Neu, C.; Sinthuprasith, T.; Sun, X.; Wang, Y.; Wolfe, E.; Xia, F.] Univ Virginia, Charlottesville, VA USA.
[Clarke, C.; Harr, R.; Karchin, P. E.; Lamichhane, P.; Sturdy, J.] Wayne State Univ, Detroit, MI USA.
[Belknap, D. A.; Dasu, S.; Dodd, L.; Duric, S.; Gomber, B.; Grothe, M.; Herndon, M.; Herve, A.; Klabbers, P.; Lanaro, A.; Levine, A.; Long, K.; Loveless, R.; Ojalvo, I.; Perry, T.; Pierro, G. A.; Polese, G.; Ruggles, T.; Savin, A.; Sharma, A.; Smith, N.; Smith, W. H.; Taylor, D.; Verwilligen, P.; Woods, N.] Univ Wisconsin Madison, Madison, WI USA.
[Fruehwirth, R.; Jeitler, M.; Schieck, J.; Wulz, C. -E.; Krammer, M.] Vienna Univ Technol, Vienna, Austria.
[Chinellato, J.] Univ Estadual Campinas, Campinas, Brazil.
[Moon, C. S.] CNRS, IN2P3, Paris, France.
Univ Libre Bruxelles, Brussels, Belgium.
[Abdelalim, A. A.] Helwan Univ, Cairo, Egypt.
[Abdelalim, A. A.] Zewail City Sci & Technol, Zewail, Egypt.
[El-khateeb, E.; Salama, E.] Ain Shams Univ, Cairo, Egypt.
[Awad, A. M. Kuotb] Fayoum Univ, Al Fayyum, Egypt.
[Salama, E.] British Univ Egypt, Cairo, Egypt.
[Petkov, P.] Univ Haute Alsace, Mulhouse, France.
[Hempel, M.] Brandenburg Tech Univ Cottbus, Cottbus, Germany.
[Horvath, D.] Inst Nucl Res ATOMKI, Debrecen, Hungary.
[Karancsi, J.] Univ Debrecen, Debrecen, Hungary.
[Choudhury, S.] Indian Inst Sci Educ & Res, Bhopal, India.
[Nayak, A.] Inst Phys, Bhubaneswar, Orissa, India.
[Bhowmik, S.; Maity, M.; Sarkar, T.] Visva Bharati Univ, Santini Ketan, W Bengal, India.
[Wickramage, N.] Univ Ruhuna, Matara, Sri Lanka.
[Chenarani, S.; Etesami, S. M.] Isfahan Univ Technol, Esfahan, Iran.
[Fahim, A.] Univ Tehran, Dept Engn Sci, Tehran, Iran.
[Safarzadeh, B.] Islamic Azad Univ, Plasma Phys Res Ctr, Sci & Res Branch, Tehran, Iran.
[Androsov, K.; Ciocci, M. A.; Grippo, M. T.] Univ Siena, Siena, Italy.
[Savoy-Navarro, A.] Purdue Univ, W Lafayette, IN USA.
[Ali, M. A. B. Md] Int Islamic Univ Malaysia, Kuala Lumpur, Malaysia.
[Idris, F. Mohamad] Agensi Nuklear Malaysia, MOSTI, Kajang, Malaysia.
[Popov, A.] Consejo Nacl Invest Cient & Tecn, Mexico City, DF, Mexico.
[Byszuk, A.; Zagozdzinska, A.] Warsaw Univ Technol, Inst Elect Syst, Warsaw, Poland.
[Matveev, V.; Musienko, Y.] Inst Nucl Res, Moscow, Russia.
[Azarkin, M.; Dremin, I.; Leonidov, A.] Natl Res Nucl Univ, Moscow Engn Phys Inst MEPhI, Moscow, Russia.
[Yuldashev, B. S.] Uzbek Acad Sci, Inst Nucl Phys, Tashkent, Uzbekistan.
[Kim, V.] St Petersburg State Polytech Univ, St Petersburg, Russia.
[Lohmann, W.; Kuznetsova, E.] Univ Florida, Gainesville, FL USA.
[Dubinin, M.] CALTECH, Pasadena, CA 91125 USA.
[Adzic, P.] Univ Belgrade, Fac Phys, Belgrade, Serbia.
[Di Marco, E.] Ist Nazl Fis Nucl, Sez Roma, Rome, Italy.
[Di Marco, E.] Univ Roma, Rome, Italy.
[Orfanelli, S.] Natl Tech Univ Athens, Athens, Greece.
[Rolandi, G.] Ist Nazl Fis Nucl, Scuola Normale & Sez, Pisa, Italy.
[Sphicas, P.] Univ Athens, Athens, Greece.
[Veckalns, V.] Riga Tech Univ, Riga, Latvia.
[Starodumov, A.; Nikitenko, A.] Inst Theoret & Expt Phys, Moscow, Russia.
[Amsler, C.] Albert Einstein Ctr Fundamental Phys, Bern, Switzerland.
[Cerci, D. Sunar; Tali, B.] Adiyaman Univ, Adiyaman, Turkey.
[Kangal, E. E.] Mersin Univ, Mersin, Turkey.
[Onengut, G.] Cag Univ, Mersin, Turkey.
[Ozdemir, K.] Piri Reis Univ, Istanbul, Turkey.
[Isildak, B.] Ozyegin Univ, Istanbul, Turkey.
[Karapinar, G.] Izmir Inst Technol, Izmir, Turkey.
[Kaya, M.] Marmara Univ, Istanbul, Turkey.
[Kaya, O.] Kafkas Univ, Kars, Turkey.
[Yetkin, E. A.] Istanbul Bilgi Univ, Istanbul, Turkey.
[Yetkin, T.] Yildiz Tech Univ, Istanbul, Turkey.
[Sen, S.] Hacettepe Univ, Ankara, Turkey.
[Newbold, D. M.; Lucas, R.] Rutherford Appleton Lab, Didcot, Oxon, England.
[Belyaev, A.] Univ Southampton, Sch Phys & Astron, Southampton, Hants, England.
[Acosta, M. Vazquez] Inst Astrofis Canarias, San Cristobal la Laguna, Spain.
[Wasserbaech, S.] Utah Valley Univ, Orem, UT USA.
[Milenovic, P.] Univ Belgrade, Fac Phys, Belgrade, Serbia.
[Milenovic, P.] Vinca Inst Nucl Sci, Belgrade, Serbia.
[Colafranceschi, S.] Univ Roma, Fac Ingn, Rome, Italy.
[Pigazzini, S.; Bilki, B.] Argonne Natl Lab, Argonne, IL USA.
[De Nardo, G.] Erzincan Univ, Erzincan, Turkey.
[Ozok, F.] Mimar Sinan Univ, Istanbul, Turkey.
[Bouhali, O.; Hernandez, A. Castaneda] Texas A&M Univ Qatar, Doha, Qatar.
[Kamon, T.] Kyungpook Natl Univ, Daegu, South Korea.
RP Khachatryan, V (reprint author), Yerevan Phys Inst, Yerevan, Armenia.
RI Azarkin, Maxim/N-2578-2015; Tuominen, Eija/A-5288-2017; Dudko,
Lev/D-7127-2012; Andreev, Vladimir/M-8665-2015; Paulini,
Manfred/N-7794-2014; Terkulov, Adel/M-8581-2015; Goh,
Junghwan/Q-3720-2016; Da Silveira, Gustavo Gil/N-7279-2014; Konecki,
Marcin/G-4164-2015; Della Ricca, Giuseppe/B-6826-2013; Ruiz,
Alberto/E-4473-2011; Manganote, Edmilson/K-8251-2013; Lokhtin,
Igor/D-7004-2012; TUVE', Cristina/P-3933-2015; Moraes,
Arthur/F-6478-2010; Puljak, Ivica/D-8917-2017; Petrushanko,
Sergey/D-6880-2012; Yazgan, Efe/C-4521-2014; Kirakosyan,
Martin/N-2701-2015; Dremin, Igor/K-8053-2015; Leonidov,
Andrey/M-4440-2013; Govoni, Pietro/K-9619-2016
OI Tuominen, Eija/0000-0002-7073-7767; Dudko, Lev/0000-0002-4462-3192;
Paulini, Manfred/0000-0002-6714-5787; Goh, Junghwan/0000-0002-1129-2083;
Da Silveira, Gustavo Gil/0000-0003-3514-7056; Konecki,
Marcin/0000-0001-9482-4841; Della Ricca, Giuseppe/0000-0003-2831-6982;
Ruiz, Alberto/0000-0002-3639-0368; TUVE', Cristina/0000-0003-0739-3153;
Moraes, Arthur/0000-0002-5157-5686; Yazgan, Efe/0000-0001-5732-7950;
Govoni, Pietro/0000-0002-0227-1301
FU BMWFW (Austria); FWF (Austria); FNRS (Belgium); FWO (Belgium); CNPq
(Brazil); CAPES (Brazil); FAPERJ (Brazil); FAPESP (Brazil); MES
(Bulgaria); CERN; CAS (China); MoST (China); NSFC (China); COL-CIENCIAS
(Colombia); MSES (Croatia); CSF (Croatia); RPF (Cyprus); MoER (Estonia);
ERC IUT (Estonia); ERDF (Estonia); Academy of Finland (Finland); MEC
(Finland); HIP (Finland); CEA (France); CNRS/IN2P3 (France); BMBF
(Germany); DFG (Germany); HGF (Germany); GSRT (Greece); OTKA (Hungary);
NIH (Hungary); DAE (India); DST (India); IPM (Iran); SFI (Ireland); INFN
(Italy); MSIP (Republic of Korea); NRF (Republic of Korea); LAS
(Lithuania); MOE (Malaysia); UM (Malaysia); CINVESTAV (Mexico); CONACYT
(Mexico); SEP (Mexico); UASLP-FAI (Mexico)
FX We congratulate our colleagues in the CERN accelerator departments for
the excellent performance of the LHC and thank the technical and
administrative staffs at CERN and at other CMS institutes for their
contributions to the success of the CMS effort. In addition, we
gratefully acknowledge the computing centers and personnel of the
Worldwide LHC Computing Grid for delivering so effectively the computing
infrastructure essential to our analyses. Finally, we acknowledge the
enduring support for the construction and operation of the LHC and the
CMS detector provided by the following funding agencies: BMWFW and FWF
(Austria); FNRS and FWO (Belgium); CNPq, CAPES, FAPERJ, and FAPESP
(Brazil); MES (Bulgaria); CERN; CAS, MoST, and NSFC (China);
COL-CIENCIAS (Colombia); MSES and CSF (Croatia); RPF (Cyprus); MoER, ERC
IUT and ERDF (Estonia); Academy of Finland, MEC, and HIP (Finland); CEA
and CNRS/IN2P3 (France); BMBF, DFG, and HGF (Germany); GSRT (Greece);
OTKA and NIH (Hungary); DAE and DST (India); IPM (Iran); SFI (Ireland);
INFN (Italy); MSIP and NRF (Republic of Korea); LAS (Lithuania); MOE and
UM (Malaysia); CINVESTAV, CONACYT, SEP, and UASLP-FAI (Mexico); MBIE
(New Zealand); PAEC (Pakistan); MSHE and NSC (Poland); FCT (Portugal);
JINR (Dubna); MON, RosAtom, RAS and RFBR (Russia); MESTD (Serbia); SEIDI
and CPAN (Spain); Swiss Funding Agencies (Switzerland); MST (Taipei);
ThEPCenter, IPST, STAR and NSTDA (Thailand); TUBITAK and TAEK (Turkey);
NASU and SFFR (Ukraine); STFC (United Kingdom); DOE and NSF (U.S.A.).
Individuals have received support from the Marie-Curie program and the
European Research Council and EPLANET (European Union); the Leventis
Foundation; the A. P. Sloan Foundation; the Alexander von Humboldt
Foundation; the Belgian Federal Science Policy Office; the Fonds pour la
Formation a la Recherche dans l'Industrie et dans l'Agriculture
(FRIA-Belgium); the Agentschap voor Innovatie door Wetenschap en
Technologie (IWT-Belgium); the Ministry of Education, Youth and Sports
(MEYS) of the Czech Republic; the Council of Science and Industrial
Research, India; the HOMING PLUS program of the Foundation for Polish
Science, cofinanced from European Union, Regional Development Fund; the
OPUS program of the National Science Center (Poland); the Compagnia di
San Paolo (Torino); MIUR project 20108T4XTM (Italy); the Thalis and
Aristeia programs cofinanced by EU-ESF and the Greek NSRF; the National
Priorities Research Program by Qatar National Research Fund; the
Rachadapisek Sompot Fund for Postdoctoral Fellowship, Chulalongkorn
University (Thailand); the Chulalongkorn Academic into Its 2nd Century
Project Advancement Project (Thailand); and the Welch Foundation,
contract C-1845.
NR 68
TC 0
Z9 0
U1 3
U2 3
PU SPRINGER
PI NEW YORK
PA 233 SPRING ST, NEW YORK, NY 10013 USA
SN 1029-8479
J9 J HIGH ENERGY PHYS
JI J. High Energy Phys.
PD OCT 3
PY 2016
IS 10
AR 006
DI 10.1007/JHEP10(2016)006
PG 61
WC Physics, Particles & Fields
SC Physics
GA DY8RH
UT WOS:000385397500001
ER
PT J
AU Aad, G
Abbott, B
Abdallah, J
Abdinov, O
Aben, R
Abolins, M
AbouZeid, OS
Abramowicz, H
Abreu, H
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Abulaiti, Y
Acharya, BS
Adamczyk, L
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Affolder, AA
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Agricola, J
Aguilar-Saavedra, JA
Ahlen, SP
Ahmadov, F
Aielli, G
Akerstedt, H
Aring;kesson, TPA
Akimov, AV
Alberghi, GL
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Verzini, MJA
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Alexander, G
Alexopoulos, T
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CA ATLAS Collaboration
TI Measurements of top-quark pair differential cross-sections in the lepton
plus jets channel in pp collisions at root s=8 TeV using the ATLAS
detector
SO EUROPEAN PHYSICAL JOURNAL C
LA English
DT Article
ID HADRON COLLIDERS; ELECTROWEAK CORRECTIONS; PARTON DISTRIBUTIONS;
RESUMMATION; LHC
AB Measurements of normalized differential cross-sections of top-quark pair production are presented as a function of the top-quark, t (t) over bar system and event-level kinematic observables in proton-proton collisions at a centre-of-mass energy of root s = 8 TeV. The observables have been chosen to emphasize the t (t) over bar production process and to be sensitive to effects of initial-and final-state radiation, to the different parton distribution functions, and to non-resonant processes and higher-order corrections. The dataset corresponds to an integrated luminosity of 20.3 fb(-1), recorded in 2012 with the ATLAS detector at the CERN Large Hadron Collider. Events are selected in the lepton+jets channel, requiring exactly one charged lepton and at least four jets with at least two of the jets tagged as originating from a b-quark. The measured spectra are corrected for detector effects and are compared to several Monte Carlo simulations. The results are in fair agreement with the predictions over a wide kinematic range. Nevertheless, most generators predict a harder top-quark transverse momentum distribution at high values than what is observed in the data. Predictions beyond NLO accuracy improve the agreement with data at high top-quark transverse momenta. Using the current settings and parton distribution functions, the rapidity distributions are not well modelled by any generator under consideration. However, the level of agreement is improved when more recent sets of parton distribution functions are used.
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[Adamczyk, L.; Bold, T.; Dabrowski, W.; Dyndal, M.; Grabowska-Bold, I.; Kisielewska, D.; Koperny, S.; Kowalski, T. Z.; Mindur, B.; Przybycien, M.; Zemla, A.] AGH Univ Sci & Technol, Fac Phys & Appl Comp Sci, Krakow, Poland.
[Palka, M.; Richter-Was, E.] Jagiellonian Univ, Marian Smoluchowski Inst Phys, Krakow, Poland.
[Banas, E.; de Renstrom, P. A. Bruckman; Chwastowski, J. J.; Derendarz, D.; Godlewski, J.; Gornicki, E.; Hajduk, Z.; Iwanski, W.; Kaczmarska, A.; Knapik, J.; Korcyl, K.; Malecki, Pa.; Olszewski, A.; Olszowska, J.; Stanecka, E.; Staszewski, R.; Trzebinski, M.; Trzupek, A.; Wolter, M. W.; Wosiek, B. K.; Wozniak, K. W.; Zabinski, B.] Polish Acad Sci, Inst Nucl Phys, Krakow, Poland.
[Cao, T.; Firan, A.; Hetherly, J. W.; Kama, S.; Kehoe, R.; Sekula, S. J.; Stroynowski, R.; Turvey, A. J.; Varol, T.; Wang, H.; Ye, J.; Zhao, X.; Zhou, L.] Southern Methodist Univ, Dept Phys, Dallas, TX USA.
[Izen, J. M.; Leyton, M.; Meirose, B.; Namasivayam, H.; Reeves, K.] Univ Texas Dallas, Dept Phys, Richardson, TX 75083 USA.
[Asbah, N.; Bessner, M.; Bloch, I.; Borroni, S.; Britzger, D.; Camarda, S.; Deterre, C.; Dutta, B.; Eckardt, C.; Filipuzzi, M.; Flaschel, N.; Glazov, A.; Gregor, I. M.; Grohsjean, A.; Haleem, M.; Hamnett, P. G.; Hengler, C.; Hiller, K. H.; Howarth, J.; Huang, Y.; Katzy, J.; Keller, J. S.; Kondrashova, N.; Kuhl, T.; Lobodzinska, E.; Lohwasser, K.; Madsen, A.; Mamuzic, J.; Medinnis, M.; Monig, K.; Garcia, R. F. Naranjo; Naumann, T.; Peschke, R.; Petit, E.; Pirumov, H.; Poley, A.; Radescu, V.; Robinson, J. E. M.; Rubinskiy, I.; Schaefer, R.; Schmitt, S.; Sedov, G.; South, D.; Stanescu-Bellu, M.; Stanitzki, M. M.; Styles, N. A.; Tackmann, K.; Wang, J.; Wasicki, C.; Yildirim, E.] DESY, Hamburg, Germany.
[Asbah, N.; Bessner, M.; Bloch, I.; Borroni, S.; Britzger, D.; Camarda, S.; Deterre, C.; Dutta, B.; Eckardt, C.; Filipuzzi, M.; Flaschel, N.; Glazov, A.; Gregor, I. M.; Grohsjean, A.; Haleem, M.; Hamnett, P. G.; Hengler, C.; Hiller, K. H.; Howarth, J.; Huang, Y.; Katzy, J.; Keller, J. S.; Kondrashova, N.; Kuhl, T.; Lobodzinska, E.; Lohwasser, K.; Madsen, A.; Mamuzic, J.; Medinnis, M.; Monig, K.; Garcia, R. F. Naranjo; Naumann, T.; Peschke, R.; Petit, E.; Pirumov, H.; Poley, A.; Radescu, V.; Robinson, J. E. M.; Rubinskiy, I.; Schaefer, R.; Schmitt, S.; Sedov, G.; South, D.; Stanescu-Bellu, M.; Stanitzki, M. M.; Styles, N. A.; Tackmann, K.; Wang, J.; Wasicki, C.; Yildirim, E.] DESY, Zeuthen, Germany.
[Burmeister, I.; Dette, K.; Erdmann, J.; Gossling, C.; Homann, M.; Jentzsch, J.; Klingenberg, R.; Kroeninger, K.] Tech Univ Dortmund, Inst Expt Phys 4, Dortmund, Germany.
[Anger, P.; Duschinger, D.; Friedrich, F.; Grohs, J. P.; Gutschow, C.; Hauswald, L.; Kobel, M.; Mader, W. F.; Novgorodova, O.; Rudolph, C.; Schnoor, U.; Siegert, F.; Socher, F.; Straessner, A.; Vest, A.; Wahrmund, S.] Tech Univ Dresden, Inst Kern & Teilchenphys, Dresden, Germany.
[Arce, A. T. H.; Benjamin, D. P.; Bjergaard, D. M.; Bocci, A.; Cerio, B. C.; Goshaw, A. T.; Kajomovitz, E.; Kotwal, A.; Kruse, M. C.; Li, L.; Li, S.; Liu, M.; Oh, S. H.; Zhou, C.] Duke Univ, Dept Phys, Durham, NC 27706 USA.
[Bristow, T. M.; Clark, P. J.; Dias, F. A.; Edwards, N. C.; Gao, Y.; Walls, F. M. Garay; Glaysher, P. C. F.; Harrington, R. D.; Leonidopoulos, C.; Martin, V. J.; Mills, C.; Pino, S. A. Olivares; Proissl, M.; Smart, B. H.; Washbrook, A.; Wynne, B. M.] Univ Edinburgh, SUPA Sch Phys & Astron, Edinburgh, Midlothian, Scotland.
[Antonelli, M.; Beretta, M.; Bilokon, H.; Chiarella, V.; Curatolo, M.; Di Nardo, R.; Esposito, B.; Gatti, C.; Giromini, P.; Laurelli, P.; Maccarrone, G.; Mancini, G.; Sansoni, A.; Testa, M.; Vilucchi, E.] Ist Nazl Fis Nucl, Lab Nazl Frascati, Frascati, Italy.
[Amoroso, S.; Arnold, H.; Boehler, M.; Bruneliere, R.; Buehrer, F.; Burgard, C. D.; Buscher, D.; Cardillo, F.; Coniavitis, E.; Consorti, V.; Dang, N. P.; Dao, V.; Di Simone, A.; Herten, G.; Jakobs, K.; Javurek, T.; Jenni, P.; Kiss, F.; Koneke, K.; Kopp, A. K.; Kuehn, S.; Landgraf, U.; Luedtke, C.; Mahboubi, K.; Mohr, W.; Pagacova, M.; Parzefall, U.; Ronzani, M.; Rosbach, K.; Ruhr, F.; Rurikova, Z.; Sammel, D.; Schillo, C.; Schumacher, M.; Sommer, P.; Sundermann, J. E.; Ta, D.; Temming, K. K.; Tsiskaridze, V.; von Radziewski, H.; Weiser, C.; Werner, M.; Zhang, L.; Zimmermann, S.] Albert Ludwigs Univ, Fak Math & Phys, Freiburg, Germany.
[Ancu, L. S.; Bell, W. H.; Noccioli, E. Benhar; De Mendizabal, J. Bilbao; Calace, N.; Clark, A.; Coccaro, A.; Delitzsch, C. M.; della Volpe, D.; Ferrere, D.; Gadomski, S.; Golling, T.; Gonzalez-Sevilla, S.; Gramling, J.; Guescini, F.; Iacobucci, G.; Katre, A.; Mermod, P.; Miucci, A.; Muenstermann, D.; Paolozzi, L.; Picazio, A.; Ristic, B.; Schramm, S.; Tykhonov, A.; Vallecorsa, S.; Wu, X.] Univ Geneva, Sect Phys, Geneva, Switzerland.
[Barberis, D.; Darbo, G.; Favareto, A.; Parodi, A. Ferretto; Gagliardi, G.; Gaudiello, A.; Gemme, C.; Guido, E.; Morettini, P.; Osculati, B.; Parodi, F.; Passaggio, S.; Rossi, L. P.; Sannino, M.; Schiavi, C.] Ist Nazl Fis Nucl, Sez Genova, Genoa, Italy.
[Barberis, D.; Favareto, A.; Parodi, A. Ferretto; Gagliardi, G.; Gaudiello, A.; Guido, E.; Osculati, B.; Parodi, F.; Sannino, M.; Schiavi, C.] Univ Genoa, Dipartimento Fis, Genoa, Italy.
[Jejelava, J.; Tskhadadze, E. G.] Iv Javakhishvili Tbilisi State Univ, E Andronikashvili Inst Phys, Tbilisi, Rep of Georgia.
[Djobava, T.; Durglishvili, A.; Khubua, J.; Mosidze, M.] Tbilisi State Univ, Inst High Energy Phys, Tbilisi, Rep of Georgia.
[Duren, M.; Kreutzfeldt, K.; Stenzel, H.] Justus Liebig Univ Giessen, Inst Phys 2, Giessen, Germany.
[Bates, R. L.; Boutle, S. K.; Madden, W. D. Breaden; Britton, D.; Buckley, A. G.; Bussey, P.; Buttar, C. M.; Buzatu, A.; Cinca, D.; D'Auria, S.; Doyle, A. T.; Ferrando, J.; de Lima, D. E. Ferreira; Gul, U.; Knue, A.; Morton, A.; Mullen, P.; O'Shea, V.; Barrera, C. Oropeza; Owen, M.; Pollard, C. S.; Qin, G.; Quilty, D.; Ravenscroft, T.; Robson, A.; St Denis, R. D.; Stewart, G. A.; Thompson, A. S.] Univ Glasgow, SUPA Sch Phys & Astron, Glasgow, Lanark, Scotland.
[Agricola, J.; Bindi, M.; Blumenschein, U.; Brandt, G.; Drechsler, E.; George, M.; Graber, L.; Grosse-Knetter, J.; Janus, M.; Kareem, M. J.; Kawamura, G.; Lai, S.; Lemmer, B.; Magradze, E.; Mantoani, M.; Mchedlidze, G.; Llacer, M. Moreno; Musheghyan, H.; Nackenhorst, O.; Nadal, J.; Quadt, A.; Rieger, J.; Schorlemmer, A. L. S.; Shabalina, E.; Stolte, P.; Weingarten, J.; Zinonos, Z.] Georg August Univ, Inst Phys 2, Gottingen, Germany.
[Albrand, S.; Collot, J.; Crepe-Renaudin, S.; Delsart, P. A.; Gabaldon, C.; Genest, M. H.; Hostachy, J-Y.; Ledroit-Guillon, F.; Lleres, A.; Lucotte, A.; Malek, F.; Monini, C.; Stark, J.; Trocme, B.; Wu, M.] Univ Grenoble Alpes, Lab Phys Subatom & Cosmol, CNRS, IN2P3, Grenoble, France.
[McFarlane, K. W.] Hampton Univ, Dept Phys, Hampton, VA 23668 USA.
[Catastini, P.; Clark, B. L.; Franklin, M.; Huth, J.; Ippolito, V.; Lazovich, T.; Mateos, D. Lopez; Mercurio, K. M.; Morii, M.; Skottowe, H. P.; Spearman, W. R.; Sun, S.; Tolley, E.; Tuna, A. N.; Yen, A. L.; Zambito, S.] Harvard Univ, Lab Particle Phys & Cosmol, Cambridge, MA 02138 USA.
[Andrei, V.; Baas, A. E.; Brandt, O.; Davygora, Y.; Djuvsland, J. I.; Dunford, M.; Geisler, M. P.; Hanke, P.; Jongmanns, J.; Kluge, E. -E.; Lang, V. S.; Meier, K.; Theenhausen, H. Meyer Zu; Villar, D. I. Narrias; Sahinsoy, M.; Scharf, V.; Schultz-Coulon, H. -C.; Stamen, R.; Starovoitov, P.; Suchek, S.; Wessels, M.] Heidelberg Univ, Kirchhoff Inst Phys, Heidelberg, Germany.
[Anders, C. F.; Giulini, M.; Kolb, M.; Lisovyi, M.; Schaetzel, S.; Schmitt, S.; Schoening, A.; Sosa, D.] Heidelberg Univ, Inst Phys, Heidelberg, Germany.
[Colombo, T.; Kretz, M.; Kugel, A.] Heidelberg Univ, ZITI Inst Tech Informat, Mannheim, Germany.
[Nagasaka, Y.] Hiroshima Inst Technol, Fac Appl Informat Sci, Hiroshima, Japan.
[Bortolotto, V.; Chan, Y. L.; Castillo, L. R. Flores; Lu, H.; Salvucci, A.; Tsui, K. M.] Chinese Univ Hong Kong, Dept Phys, Shatin, Hong Kong, Peoples R China.
[Bortolotto, V.] Univ Hong Kong, Dept Phys, Pokfulam, Hong Kong, Peoples R China.
[Bortolotto, V.; Prokofiev, K.] Hong Kong Univ Sci & Technol, Dept Phys, Kowloon, Hong Kong, Peoples R China.
[Choi, K.; Dattagupta, A.; Evans, H.; Gagnon, P.; Lammers, S.; Martinez, N. Lorenzo; Luehring, F.; Ogren, H.; Penwell, J.; Weinert, B.; Zieminska, D.] Indiana Univ, Dept Phys, Bloomington, IN 47405 USA.
[Jansky, R.; Kneringer, E.; Lukas, W.; Usanova, A.; Vigne, R.] Leopold Franzens Univ, Inst Astro & Teilchenphys, Innsbruck, Austria.
[Argyropoulos, S.; Mallik, U.; Mandrysch, R.; Zaidan, R.] Univ Iowa, Iowa City, IA USA.
[Chen, C.; Cochran, J.; De Lorenzi, F.; Krumnack, N.; Pluth, D.; Prell, S.] Iowa State Univ, Dept Phys & Astron, Ames, IA USA.
[Ahmadov, F.; Aleksandrov, I. N.; Bednyakov, V. A.; Boyko, I. R.; Budagov, I. A.; Chelkov, G. A.; Cheplakov, A.; Chizhov, M. V.; Dedovich, D. V.; Demichev, M.; Gostkin, M. I.; Huseynov, N.; Javadov, N.; Karpov, S. N.; Karpova, Z. M.; Khramov, E.; Kotov, V. M.; Kruchonak, U.; Kukhtin, V.; Ladygin, E.; Minashvili, I. A.; Mineev, M.; Peshekhonov, V. D.; Plotnikova, E.; Potrap, I. N.; Pozdnyakov, V.; Rusakovich, N. A.; Sadykov, R.; Sapronov, A.; Shiyakova, M.; Sisakyan, A. N.; Soloshenko, A.; Vinogradov, V. B.; Yeletskikh, I.; Zhemchugov, A.; Zimine, N. I.] JINR Dubna, Joint Inst Nucl Res, Dubna, Russia.
[Amako, K.; Aoki, M.; Arai, Y.; Hanagaki, K.; Ikegami, Y.; Ikeno, M.; Iwasaki, H.; Kanzaki, J.; Kohriki, T.; Kondo, T.; Kono, T.; Makida, Y.; Nagano, K.; Nakamura, K.; Nozaki, M.; Odaka, S.; Okuyama, T.; Sasaki, O.; Suzuki, S.; Takubo, Y.; Tanaka, S.; Terada, S.; Tokushuku, K.; Tsuno, S.; Unno, Y.; Yamada, M.; Yamamoto, A.; Yasu, Y.] KEK, High Energy Accelerator Res Org, Tsukuba, Ibaraki, Japan.
[Chen, Y.; Hasegawa, M.; Kido, S.; Kishimoto, T.; Kurashige, H.; Maeda, J.; Shimizu, S.; Takeda, H.; Yakabe, R.; Yamazaki, Y.; Yuan, L.] Kobe Univ, Grad Sch Sci, Kobe, Hyogo, Japan.
[Ishino, M.; Kunigo, T.; Monden, R.; Sumida, T.; Tashiro, T.] Kyoto Univ, Fac Sci, Kyoto, Japan.
[Takashima, R.] Kyoto Univ, Kyoto, Japan.
[Kawagoe, K.; Oda, S.; Otono, H.; Tojo, J.] Kyushu Univ, Dept Phys, Fukuoka, Japan.
[Verzini, M. J. Alconada; Alonso, F.; Arduh, F. A.; Dova, M. T.; Monticelli, F.; Wahlberg, H.] Univ Nacl La Plata, Inst Fis La Plata, La Plata, Buenos Aires, Argentina.
[Verzini, M. J. Alconada; Alonso, F.; Arduh, F. A.; Dova, M. T.; Monticelli, F.; Wahlberg, H.] Consejo Nacl Invest Cient & Tecn, La Plata, Buenos Aires, Argentina.
[Barton, A. E.; Beattie, M. D.; Borissov, G.; Bouhova-Thacker, E. V.; Dearnaley, W. J.; Fox, H.; Grimm, K.; Henderson, R. C. W.; Hughes, G.; Jones, R. W. L.; Kartvelishvili, V.; Long, R. E.; Love, P. A.; Maddocks, H. J.; Skinner, M. B.; Smizanska, M.; Walder, J.; Wharton, A. M.] Univ Lancaster, Dept Phys, Lancaster, England.
[Chiodini, G.; Gorini, E.; Primavera, M.; Spagnolo, S.; Ventura, A.] INFN, Sez Lecce, Lecce, Italy.
[Gorini, E.; Spagnolo, S.; Ventura, A.] Univ Salento, Dipartimento Matemat & Fis, Lecce, Italy.
[Affolder, A. A.; Anders, J. K.; Burdin, S.; D'Onofrio, M.; Dervan, P.; Gwilliam, C. B.; Hayward, H. S.; Jones, T. J.; King, B. T.; Klein, M.; Klein, U.; Kretzschmar, J.; Laycock, P.; Lehan, A.; Maxfield, S. J.; Mehta, A.; Readioff, N. P.; Schnellbach, Y. J.; Vossebeld, J. H.] Univ Liverpool, Oliver Lodge Lab, Liverpool, Merseyside, England.
[Cindro, V.; Deliyergiyev, M.; Filipcic, A.; Gorisek, A.; Kersevan, B. P.; Kramberger, G.; Macek, B.; Mandic, I.; Mikuz, M.; Sfiligoj, T.; Sokhrannyi, G.] Jozef Stefan Inst, Dept Phys, Ljubljana, Slovenia.
[Cindro, V.; Deliyergiyev, M.; Filipcic, A.; Gorisek, A.; Kersevan, B. P.; Kramberger, G.; Macek, B.; Mandic, I.; Mikuz, M.; Sfiligoj, T.; Sokhrannyi, G.] Univ Ljubljana, Ljubljana, Slovenia.
[Bevan, A. J.; Bona, M.; Cerrito, L.; Fletcher, G.; Goddard, J. R.; Hays, J. M.; Hickling, R.; Landon, M. P. J.; Lloyd, S. L.; Morris, J. D.; Nooney, T.; Piccaro, E.; Rizvi, E.; Sandbach, R. L.; Snidero, G.; Castanheira, M. Teixeira Dias] Queen Mary Univ London, Sch Phys & Astron, London, England.
[Berry, T.; Blanco, J. E.; Boisvert, V.; Brooks, T.; Connelly, I. A.; Cowan, G.; Duguid, L.; Giannelli, M. Faucci; George, S.; Gibson, S. M.; Kempster, J. J.; Vazquez, J. G. Panduro; Pastore, Fr.; Savage, G.; Sowden, B. C.; Spano, F.; Teixeira-Dias, P.; Thomas-Wilsker, J.] Royal Holloway Univ London, Dept Phys, Surrey, England.
[Butterworth, J. M.; Campanelli, M.; Casadei, D.; Chislett, R. T.; Christodoulou, V.; Cooper, B. D.; Davison, P.; Falla, R. J.; Freeborn, D.; Gregersen, K.; Ortiz, N. G. Gutierrez; Hesketh, G. G.; Jansen, E.; Jiggins, S.; Konstantinidis, N.; Korn, A.; Kucuk, H.; Lambourne, L.; Leney, K. J. C.; Martyniuk, A. C.; Mcfayden, J. A.; Nurse, E.; Richter, S.; Scanlon, T.; Sherwood, P.; Simmons, B.; Wardrope, D. R.; Waugh, B. M.] UCL, Dept Phys & Astron, London, England.
[Greenwood, Z. D.; Grossi, G. C.; Jana, D. K.; Sawyer, L.; Subramaniam, R.] Louisiana Tech Univ, Ruston, LA 71270 USA.
[Beau, T.; Bomben, M.; Calderini, G.; Crescioli, F.; De Cecco, S.; Demilly, A.; Derue, F.; Francavilla, P.; Krasny, M. W.; Lacour, D.; Laforge, B.; Laplace, S.; Le Dortz, O.; Lefebvre, G.; Malaescu, B.; Marchiori, G.; Nikolic-Audit, I.; Ocariz, J.; Pandini, C. E.; Pires, S.; Ridel, M.; Roos, L.; Trincaz-Duvoid, S.; Vannucci, F.; Varouchas, D.; Yap, Y. C.] UPMC, Lab Phys Nucl & Hautes Energies, Paris, France.
[Beau, T.; Bomben, M.; Calderini, G.; Crescioli, F.; De Cecco, S.; Demilly, A.; Derue, F.; Francavilla, P.; Krasny, M. W.; Lacour, D.; Laforge, B.; Laplace, S.; Le Dortz, O.; Lefebvre, G.; Malaescu, B.; Marchiori, G.; Nikolic-Audit, I.; Ocariz, J.; Pandini, C. E.; Pires, S.; Ridel, M.; Roos, L.; Trincaz-Duvoid, S.; Vannucci, F.; Varouchas, D.; Yap, Y. C.] Univ Paris Diderot, Paris, France.
[Beau, T.; Bomben, M.; Calderini, G.; Crescioli, F.; De Cecco, S.; Demilly, A.; Derue, F.; Francavilla, P.; Krasny, M. W.; Lacour, D.; Laforge, B.; Laplace, S.; Le Dortz, O.; Lefebvre, G.; Malaescu, B.; Marchiori, G.; Nikolic-Audit, I.; Ocariz, J.; Pandini, C. E.; Pires, S.; Ridel, M.; Roos, L.; Trincaz-Duvoid, S.; Vannucci, F.; Varouchas, D.; Yap, Y. C.] CNRS, IN2P3, Paris, France.
[Akesson, T. P. A.; Bocchetta, S. S.; Bryngemark, L.; Doglioni, C.; Floderus, A.; Hawkins, A. D.; Hedberg, V.; Ivarsson, J.; Jarlskog, G.; Lytken, E.; Mjornmark, J. U.; Smirnova, O.; Viazlo, O.] Lund Univ, Fys Inst, Lund, Sweden.
[Barreiro, F.; Cantero, J.; De la Torre, H.; Del Peso, J.; Glasman, C.; Merino, J. Llorente; Terron, J.] Univ Autonoma Madrid, Dept Fis Teor C15, Madrid, Spain.
[Artz, S.; Becker, M.; Bertella, C.; Blum, W.; Buscher, V.; Caputo, R.; Caudron, J.; Cuth, J.; Endner, O. C.; Ertel, E.; Fiedler, F.; Torregrosa, E. Fullana; Groh, S.; Heck, T.; Hohlfeld, M.; Hulsing, T. A.; Jakobi, K. B.; Kaluza, A.; Karnevskiy, M.; Kleinknecht, K.; Kopke, L.; Lin, T. H.; Masetti, L.; Mattmann, J.; Meyer, C.; Moritz, S.; Rave, S.; Sander, H. G.; Schaeffer, J.; Schafer, U.; Schmitt, C.; Schmitz, S.; Schott, M.; Schuh, N.; Simioni, E.; Simon, M.; Tapprogge, S.; Valderanis, C.; Wollstadt, S. J.; Zimmermann, C.; Zinser, M.] Johannes Gutenberg Univ Mainz, Inst Phys, Mainz, Germany.
[Balli, F.; Barnes, S. L.; Cox, B. E.; Da Via, C.; Forti, A.; Ponce, J. M. Iturbe; Joshi, K. D.; Keoshkerian, H.; Li, X.; Loebinger, F. K.; Marsden, S. P.; Masik, J.; Sanchez, F. J. Munoz; Neep, T. J.; Oh, A.; Ospanov, R.; Pater, J. R.; Peters, R. F. Y.; Pilkington, A. D.; Pin, A. W. J.; Price, D.; Qin, Y.; Queitsch-Maitland, M.; Schwanenberger, C.; Schweiger, H.; Shaw, S. M.; Thompson, R. J.; Tomlinson, L.; Watts, S.; Webb, S.; Woudstra, M. J.; Wyatt, T. R.] Univ Manchester, Sch Phys & Astron, Manchester, Lancs, England.
[Aad, G.; Alio, L.; Barbero, M.; Coadou, Y.; Diaconu, C.; Diglio, S.; Djama, F.; Ducu, O. A.; Feligioni, L.; Gao, J.; Hallewell, G. D.; Hubaut, F.; Kahn, S. J.; Knoops, E. B. F. G.; Le Guirriec, E.; Liu, J.; Liu, K.; Madaffari, D.; Mochizuki, K.; Monnier, E.; Muanza, S.; Nagai, Y.; Nagy, E.; Pralavorio, P.; Rozanov, A.; Serre, T.; Talby, M.; Torres, R. E. Ticse; Tiouchichine, E.; Tisserant, S.; Toth, J.; Touchard, F.; Vacavant, L.] MAix Marseille Univ, CPP, Marseille, France.
[Aad, G.; Alio, L.; Barbero, M.; Coadou, Y.; Diaconu, C.; Diglio, S.; Djama, F.; Ducu, O. A.; Feligioni, L.; Gao, J.; Hallewell, G. D.; Hubaut, F.; Kahn, S. J.; Knoops, E. B. F. G.; Le Guirriec, E.; Liu, J.; Liu, K.; Madaffari, D.; Mochizuki, K.; Monnier, E.; Muanza, S.; Nagai, Y.; Nagy, E.; Pralavorio, P.; Rozanov, A.; Serre, T.; Talby, M.; Torres, R. E. Ticse; Tiouchichine, E.; Tisserant, S.; Toth, J.; Touchard, F.; Vacavant, L.] CNRS, IN2P3, Marseille, France.
[Bellomo, M.; Bernard, N. R.; Brau, B.; Dallapiccola, C.; Daya-Ishmukhametova, R. K.; Moyse, E. J. W.; Pais, P.; Pueschel, E.; Ventura, D.; Willocq, S.] Univ Massachusetts, Dept Phys, Amherst, MA 01003 USA.
[Belanger-Champagne, C.; Chuinard, A. J.; Corriveau, F.; Keyes, R. A.; Mantifel, R.; Prince, S.; Robertson, S. H.; Robichaud-Veronneau, A.; Stockton, M. C.; Stoebe, M.; Vachon, B.; Schroeder, T. Vazquez; Wang, K.; Warburton, A.] McGill Univ, Dept Phys, Montreal, PQ, Canada.
[Barberio, E. L.; Brennan, A. J.; Dawe, E.; Jennens, D.; Kubota, T.; Milesi, M.; Hanninger, G. Nunes; Nuti, F.; Rados, P.; Spiller, L. A.; Tan, K. G.; Taylor, G. N.; Taylor, P. T. E.; Ungaro, F. C.; Urquijo, P.; Volpi, M.; Zanzi, D.] Univ Melbourne, Sch Phys, Melbourne, Vic, Australia.
[Amidei, D.; Chelstowska, M. A.; Cheng, H. C.; Dai, T.; Diehl, E. B.; Edgar, R. C.; Feng, H.; Ferretti, C.; Fleischmann, P.; Goldfarb, S.; Guan, L.; Hu, X.; Levin, D.; Liu, H.; Lu, N.; Marley, D. E.; McKee, S. P.; McCarn, A.; Neal, H. A.; Qian, J.; Schwarz, T. A.; Searcy, J.; Sekhon, K.; Thun, R. P.; Wilson, A.; Wu, Y.; Yu, J. M.; Zhang, D.; Zhou, B.; Zhu, J.] Univ Michigan, Dept Phys, Ann Arbor, MI 48109 USA.
[Abolins, M.; Arabidze, G.; Brock, R.; Chegwidden, A.; Fisher, W. C.; Halladjian, G.; Hauser, R.; Hayden, D.; Huston, J.; Linnemann, J. T.; Martin, B.; Mondragon, M. C.; Pope, B. G.; Schoenrock, B. D.; Schwienhorst, R.; Tollefson, K.; Willis, C.] Michigan State Univ, Dept Phys & Astron, E Lansing, MI 48824 USA.
[Alimonti, G.; Andreazza, A.; Besana, M. I.; Carminati, L.; Cavalli, D.; Costa, G.; Fanti, M.; Giugni, D.; Lari, T.; Mandelli, L.; Mazza, S. M.; Meroni, C.; Perini, L.; Pizio, C.; Ragusa, F.; Resconi, S.; Shojaii, S.; Stabile, A.; Tartarelli, G. F.; Troncon, C.; Turra, R.; Perez, M. Villaplana] INFN, Sez Milano, Milan, Italy.
[Andreazza, A.; Fanti, M.; Mazza, S. M.; Perini, L.; Pizio, C.; Ragusa, F.; Shojaii, S.; Turra, R.; Perez, M. Villaplana] Univ Milan, Dipartimento Fis, Milan, Italy.
[Carminati, L.; Harkusha, S.; Kulchitsky, Y.; Kurochkin, Y. A.; Tsiareshka, P. V.] Natl Acad Sci Belarus, BI Stepanov Inst Phys, Minsk, Byelarus.
[Hrynevich, A.] Natl Sci & Educ Ctr Particle & High Energy Phys, Minsk, Byelarus.
[Taylor, F. E.] MIT, Dept Phys, Cambridge, MA 02139 USA.
[Arguin, J-F.; Azuelos, G.; Dallaire, F.; Gauthier, L.; Leroy, C.; Rezvani, R.; Saadi, D. Shoaleh] Univ Montreal, Grp Particle Phys, Montreal, PQ, Canada.
[Akimov, A. V.; Gavrilenko, I. L.; Komar, A. A.; Mashinistov, R.; Mouraviev, S. V.; Nechaeva, P. Yu.; Shmeleva, A.; Snesarev, A. A.; Sulin, V. V.; Tikhomirov, V. O.; Zhukov, K.] Russian Acad Sci, PN Lebedev Phys Inst, Moscow, Russia.
[Artamonov, A.; Gorbounov, P. A.; Khovanskiy, V.; Shatalov, P. B.; Tsukerman, I.] Inst Theoret & Expt Phys ITEP, Moscow, Russia.
[Antonov, A.; Belotskiy, K.; Bulekov, O.; Dolgoshein, B. A.; Kantserov, V. A.; Krasnopevtsev, D.; Romaniouk, A.; Shulga, E.; Smirnov, S. Yu.; Smirnov, Y.; Soldatov, E. Yu.; Timoshenko, S.; Vorobev, K.] Natl Res Nucl Univ MEPhI, Moscow, Russia.
[Boldyrev, A. S.; Gladilin, L. K.; Kramarenko, V. A.; Maevskiy, A.; Rud, V. I.; Sivoklokov, S. Yu.; Smirnova, L. N.; Turchikhin, S.] Moscow MV Lomonosov State Univ, DV Skobeltsyn Inst Nucl Phys, Moscow, Russia.
[Adomeit, S.; Bender, M.; Biebel, O.; Bock, C.; Bortfeldt, J.; Calfayan, P.; Chow, B. K. B.; Duckeck, G.; Elmsheuser, J.; Hertenberger, R.; Hoenig, F.; Legger, F.; Lorenz, J.; Losel, P. J.; Maier, T.; Mann, A.; Mehlhase, S.; Meineck, C.; Mitrevski, J.; Mueller, R. S. P.; Nunnemann, T.; Rauscher, F.; Ruschke, A.; Sanders, M. P.; Schaile, D.; Unverdorben, C.; Vladoiu, D.; Walker, R.; Wittkowski, J.] Ludwig Maximilians Univ Munchen, Fak Phys, Munich, Germany.
[Barillari, T.; Bethke, S.; Bronner, J.; Compostella, G.; Cortiana, G.; Ecker, K. M.; Flowerdew, M. J.; Giuliani, C.; Goblirsch-Kolb, M.; Ince, T.; Kiryunin, A. E.; Kluth, S.; Kortner, O.; Kortner, S.; Kroha, H.; Macchiolo, A.; Maier, A. A.; Menke, S.; Mueller, F.; Nagel, M.; Nisius, R.; Nowak, S.; Oberlack, H.; Richter, R.; Salihagic, D.; Sandstroem, R.; Schacht, P.; Schwegler, Ph.; Spettel, F.; Stonjek, S.; Terzo, S.; von der Schmitt, H.; Wildauer, A.] Max Planck Inst Phys & Astrophys, Werner Heisenberg Inst, Munich, Germany.
[Fusayasu, T.; Shimojima, M.] Nagasaki Inst Appl Sci, Nagasaki, Japan.
[Horii, Y.; Kawade, K.; Morvaj, L.; Onogi, K.; Tomoto, M.; Wakabayashi, J.; Yamauchi, K.] Nagoya Univ, Grad Sch Sci, Nagoya, Aichi, Japan.
[Horii, Y.; Kawade, K.; Morvaj, L.; Onogi, K.; Tomoto, M.; Wakabayashi, J.; Yamauchi, K.] Nagoya Univ, Kobayashi Maskawa Inst, Nagoya, Aichi, Japan.
[Aloisio, A.; Alviggi, M. G.; Canale, V.; Carlino, G.; Cirotto, F.; Conventi, F.; de Asmundis, R.; Della Pietra, M.; Doria, A.; Izzo, V.; Merola, L.; Perrella, S.; Rossi, E.; Sanchez, A.; Sekhniaidze, G.; Zurzolo, G.] INFN, Sez Napoli, Naples, Italy.
[Aloisio, A.; Alviggi, M. G.; Canale, V.; Cirotto, F.; Merola, L.; Perrella, S.; Rossi, E.; Sanchez, A.; Zurzolo, G.] Univ Napoli, Dipartimento Fis, Naples, Italy.
[Gorelov, I.; Hoeferkamp, M. R.; Seidel, S. C.; Taylor, A. C.; Toms, K.] Univ New Mexico, Dept Phys & Astron, Albuquerque, NM 87131 USA.
[Caron, S.; Colasurdo, L.; Croft, V.; De Groot, N.; Filthaut, F.; Galea, C.; Konig, A. C.; Nektarijevic, S.; Strubig, A.] Radboud Univ Nijmegen, Inst Math Astrophys & Particle Phys, Nikhef, Nijmegen, Netherlands.
[Deigaard, I.; Deluca, C.; Duda, D.; Hartjes, F.; Linde, F.; Mahlstedt, J.; Meyer, J.; Oussoren, K. P.; Sabato, G.; Salek, D.; van der Graaf, H.; van Vulpen, I.; Vermeulen, J. C.; Weits, H.] Nikhef Natl Inst Subat Phys, Amsterdam, Netherlands.
[Aben, R.; Angelozzi, I.; Beemster, L. J.; Bentvelsen, S.; Berge, D.; Bobbink, G. J.; Bos, K.; Brenner, L.; Butti, P.; Castelli, A.; Colijn, A. P.; de Jong, P.; Deigaard, I.; Deluca, C.; Duda, D.; Ferrari, P.; Hartjes, F.; Hessey, N. P.; Hod, N.; Igonkina, O.; Karastathis, N.; Kluit, P.; Koffeman, E.; Linde, F.; Mahlstedt, J.; Meyer, J.; Oussoren, K. P.; Sabato, G.; Salek, D.; Slawinska, M.; Valencic, N.; Van den Wollenberg, W.; Van der Deijl, P. C.; van der Geer, R.; van der Graaf, H.; van Vulpen, I.; Verkerke, W.; Vermeulen, J. C.; Vreeswijk, M.; Weits, H.; Williams, S.] Univ Amsterdam, Amsterdam, Netherlands.
[Adelman, J.; Andari, N.; Burghgrave, B.; Chakraborty, D.; Cole, S.; Saha, P.; Yurkewicz, A.] Northern Illinois Univ, Dept Phys, De Kalb, IL USA.
[Anisenkov, A. V.; Baldin, E. M.; Bobrovnikov, V. S.; Bogdanchikov, A. G.; Buzykaev, A. R.; Kazanin, V. F.; Kharlamov, A. G.; Korol, A. A.; Malyshev, V. M.; Maslennikov, A. L.; Maximov, D. A.; Peleganchuk, S. V.; Rezanova, O. L.; Soukharev, A. M.; Talyshev, A. A.; Tikhonov, Yu. A.] RAS, Budker Inst Nucl Phys, SB, Novosibirsk, Russia.
[Bernius, C.; Cranmer, K.; Haas, A.; Heinrich, L.; Kaplan, B.; Karthik, K.; Konoplich, R.; Kreiss, S.; Mincer, A. I.; Nemethy, P.; Neves, R. M.] NYU, Dept Phys, 4 Washington Pl, New York, NY 10003 USA.
[Beacham, J. B.; Gan, K. K.; Ishmukhametov, R.; Kagan, H.; Kass, R. D.; Looper, K. A.; Nagarkar, A.; Pignotti, D. T.; Shrestha, S.; Tannenwald, B. B.] Ohio State Univ, Columbus, OH 43210 USA.
[Nakano, I.] Okayama Univ, Fac Sci, Okayama, Japan.
[Abbott, B.; Alhroob, M.; Bertsche, C.; Bertsche, D.; De Benedetti, A.; Gutierrez, P.; Hasib, A.; Norberg, S.; Pearson, B.; Rifki, O.; Saleem, M.; Severini, H.; Skubic, P.; Strauss, M.] Univ Oklahoma, Homer L Dodge Dept Phys & Astron, Norman, OK 73019 USA.
[Bousson, N.; Haley, J.; Jamin, D. . O.; Khanov, A.; Rizatdinova, F.; Sidorov, D.; Yu, J.] Oklahoma State Univ, Dept Phys, Stillwater, OK 74078 USA.
[Chytka, L.; Hamal, P.; Hrabovsky, M.; Kvita, J.; Nozka, L.] Palacky Univ, RCPTM, Olomouc, Czech Republic.
[Abreu, R.; Brau, J. E.; Brost, E.; Hopkins, W. H.; Majewski, S.; Potter, C. T.; Ptacek, E.; Radloff, P.; Shamim, M.; Sinev, N. B.; Strom, D. M.; Torrence, E.; Wanotayaroj, C.; Whalen, K.; Winklmeier, F.] Univ Oregon, Ctr High Energy Phys, Eugene, OR 97403 USA.
[Ayoub, M. K.; Bassalat, A.; Becot, C.; Binet, S.; Bourdarios, C.; De Regie, J. B. De Vivie; Delgove, D.; Duflot, L.; Escalier, M.; Fayard, L.; Fournier, D.; Gkougkousis, E. L.; Grivaz, J. -F; Guillemin, T.; Hariri, F.; Henrot-Versille, S.; Hrivnac, J.; Iconomidou-Fayard, L.; Kado, M.; Lounis, A.; Makovec, N.; Morange, N.; Nellist, C.; Petroff, P.; Poggioli, L.; Puzo, P.; Renaud, A.; Rousseau, D.; Rybkin, G.; Schaffer, A. C.; Scifo, E.; Serin, L.; Simion, S.; Tanaka, R.; Zerwas, D.; Zhang, Z.; Zhao, Y.] Univ Paris Saclay, LAL, Univ Paris Sud, CNRS,IN2P3, Orsay, France.
[Endo, M.; Nomachi, M.; Okamura, W.; Sugaya, Y.; Teoh, J. J.; Yamaguchi, Y.] Osaka Univ, Grad Sch Sci, Osaka, Japan.
[Bugge, L.; Bugge, M. K.; Cameron, D.; Catmore, J. R.; Franconi, L.; Garonne, V.; Gjelsten, B. K.; Gramstad, E.; Morisbak, V.; Nilsen, J. K.; Ould-Saada, F.; Pajchel, K.; Pedersen, M.; Raddum, S.; Read, A. L.; Rohne, O.; Sandaker, H.; Stapnes, S.; Strandlie, A.] Univ Oslo, Dept Phys, Oslo, Norway.
[Barr, A. J.; Becker, K.; Behr, J. K.; Beresford, L.; Cooper-Sarkar, A. M.; Ortuzar, M. Crispin; Dafinca, A.; Davies, E.; Frost, J. A.; Gallas, E. J.; Gupta, S.; Gwenlan, C.; Hall, D.; Hays, C. P.; Henderson, J.; Howard, J.; Huffman, T. B.; Issever, C.; Kalderon, C. W.; Kogan, L. A.; Lewis, A.; Nagai, K.; Nickerson, R. B.; Pickering, M. A.; Ryder, N. C.; Tseng, J. C-L.; Viehhauser, G. H. A.; Weidberg, A. R.; Zhong, J.] Univ Oxford, Dept Phys, Oxford, England.
[Conta, C.; Dondero, P.; Ferrari, R.; Fraternali, M.; Gaudio, G.; Introzzi, G.; Lanza, A.; Livan, M.; Negri, A.; Polesello, G.; Rebuzzi, D. M.; Rimoldi, A.; Vercesi, V.] INFN, Sez Pavia, Pavia, Italy.
[Conta, C.; Dondero, P.; Fraternali, M.; Introzzi, G.; Livan, M.; Negri, A.; Rebuzzi, D. M.; Rimoldi, A.] Univ Pavia, Dipartimento Fis, Pavia, Italy.
[Balunas, W. K.; Brendlinger, K.; Fletcher, R. R. M.; Haney, B.; Heim, S.; Hines, E.; Jackson, B.; Kroll, J.; Lipeles, E.; Miguens, J. Machado; Meyer, C.; Mistry, K. P.; Reichert, J.; Stahlman, J.; Thomson, E.; Vanguri, R.; Williams, H. H.; Yoshihara, K.] Univ Penn, Dept Phys, Philadelphia, PA 19104 USA.
[Basalaev, A.; Ezhilov, A.; Fedin, O. L.; Gratchev, V.; Levchenko, M.; Maleev, V. P.; Ryabov, Y. F.; Schegelsky, V. A.; Sedykh, E.; Seliverstov, D. M.; Solovyev, V.] Natl Res Ctr, Kurchatov Inst, BP Konstantinov Petersburg Nucl Physics Inst, St Petersburg, Russia.
[Annovi, A.; Beccherle, R.; Bertolucci, F.; Biesuz, N. V.; Cavasinni, V.; Chiarelli, G.; Del Prete, T.; Dell'Orso, M.; Donati, S.; Giannetti, P.; Leone, S.; Roda, C.; Scuri, F.; Sotiropoulou, C. L.; Spalla, M.; Volpi, G.; White, S.] INFN, Sez Pisa, Pisa, Italy.
[Annovi, A.; Beccherle, R.; Bertolucci, F.; Biesuz, N. V.; Cavasinni, V.; Chiarelli, G.; Del Prete, T.; Dell'Orso, M.; Donati, S.; Giannetti, P.; Leone, S.; Roda, C.; Scuri, F.; Sotiropoulou, C. L.; Spalla, M.; Volpi, G.; White, S.] Univ Pisa, Dipartimento Fis E Fermi, Pisa, Italy.
[Bianchi, R. M.; Boudreau, J.; Escobar, C.; Hong, T. M.; Mueller, J.; Sapp, K.; Su, J.] Univ Pittsburgh, Dept Phys & Astron, Pittsburgh, PA 15260 USA.
[Aguilar-Saavedra, J. A.; Dos Santos, S. P. Amor; Amorim, A.; Araque, J. P.; Cantrill, R.; Carvalho, J.; Castro, N. F.; Muino, P. Conde; De Sousa, M. J. Da Cunha Sargedas; Fiolhais, M. C. N.; Galhardo, B.; Gomes, A.; Goncalo, R.; Jorge, P. M.; Lopes, L.; Maio, A.; Maneira, J.; Onofre, A.; Palma, A.; Pedro, R.; Pina, J.; Santos, H.; Saraiva, J. G.; Silva, J.; Delgado, A. Tavares; Veloso, F.; Wolters, H.] Lab Instrumentacao & Fis Expt Particulas LIP, Lisbon, Portugal.
[Amorim, A.; Muino, P. Conde; De Sousa, M. J. Da Cunha Sargedas; Gomes, A.; Jorge, P. M.; Miguens, J. Machado; Maio, A.; Maneira, J.; Palma, A.; Pedro, R.; Pina, J.; Delgado, A. Tavares] Univ Lisbon, Fac Ciencias, Lisbon, Portugal.
[Dos Santos, S. P. Amor; Carvalho, J.; Fiolhais, M. C. N.; Galhardo, B.; Veloso, F.; Wolters, H.] Univ Coimbra, Dept Phys, Coimbra, Portugal.
[Gomes, A.; Maio, A.; Pina, J.; Saraiva, J. G.; Silva, J.] Univ Lisbon, Ctr Fis Nucl, Lisbon, Portugal.
[Onofre, A.] Univ Minho, Dept Fis, Braga, Portugal.
[Aguilar-Saavedra, J. A.] Univ Granada, Dept Fis Teor & Cosmos, Granada, Spain.
[Aguilar-Saavedra, J. A.] Univ Granada, CAFPE, Granada, Spain.
Univ Nova Lisboa, Dep Fis, Caparica, Portugal.
Univ Nova Lisboa, CEFITEC, Fac Ciencias & Tecnol, Caparica, Portugal.
[Chudoba, J.; Havranek, M.; Hejbal, J.; Jakoubek, T.; Kepka, O.; Kupco, A.; Kus, V.; Lokajicek, M.; Lysak, R.; Marcisovsky, M.; Mikestikova, M.; Nemecek, S.; Penc, O.; Sicho, P.; Staroba, P.; Svatos, M.; Tasevsky, M.; Vrba, V.] Acad Sci Czech Republic, Inst Phys, Prague, Czech Republic.
[Augsten, K.; Caforio, D.; Gallus, P.; Guenther, J.; Hubacek, Z.; Jakubek, J.; Kohout, Z.; Myska, M.; Pospisil, S.; Seifert, F.; Simak, V.; Slavicek, T.; Smolek, K.; Solar, M.; Solc, J.; Sopczak, A.; Sopko, B.; Sopko, V.; Suk, M.; Turecek, D.; Vacek, V.; Vlasak, M.; Vokac, P.; Vykydal, Z.; Zeman, M.] Czech Tech Univ, Prague, Czech Republic.
[Balek, P.; Berta, P.; Cerny, K.; Chalupkova, I.; Davidek, T.; Dolejsi, J.; Dolezal, Z.; Faltova, J.; Kodys, P.; Kosek, T.; Leitner, R.; Pleskot, V.; Reznicek, P.; Scheirich, D.; Spousta, M.; Sykora, T.; Tas, P.; Todorova-Nova, S.; Valkar, S.; Vorobel, V.] Charles Univ Prague, Fac Math & Phys, Prague, Czech Republic.
[Borisov, A.; Cheremushkina, E.; Denisov, S. P.; Fakhrutdinov, R. M.; Fenyuk, A. B.; Golubkov, D.; Kamenshchikov, A.; Karyukhin, A. N.; Kozhin, A. S.; Minaenko, A. A.; Myagkov, A. G.; Nikolaenko, V.; Ryzhov, A.; Solodkov, A. A.; Solovyanov, O. V.; Starchenko, E. A.; Zaitsev, A. M.; Zenin, O.] NRC KI, State Res Ctr Inst High Energy Phys Protvino, Protvino, Russia.
[Baines, J. T.; Barnett, B. M.; Burke, S.; Dewhurst, A.; Dopke, J.; Emeliyanov, D.; Gallop, B. J.; Gee, C. N. P.; Haywood, S. J.; Kirk, J.; Martin-Haugh, S.; McCubbin, N. A.; McMahon, S. J.; Middleton, R. P.; Murray, W. J.; Phillips, P. W.; Sankey, D. P. C.; Sawyer, C.; Tyndel, M.; Wickens, F. J.; Wielers, M.] Rutherford Appleton Lab, Particle Phys Dept, Didcot, Oxon, England.
[Anulli, F.; Bagiacchi, P.; Bagnaia, P.; Bauce, M.; Bini, C.; Ciapetti, G.; De Pedis, D.; De Salvo, A.; Di Domenico, A.; Di Donato, C.; Falciano, S.; Gauzzi, P.; Gentile, S.; Giagu, S.; Gustavino, G.; Kuna, M.; Lacava, F.; Luci, C.; Luminari, L.; Marzano, F.; Messina, A.; Monzani, S.; Nisati, A.; Pasqualucci, E.; Petrolo, E.; Pontecorvo, L.; Rescigno, M.; Rosati, S.; Tehrani, F. Safai; Vanadia, M.; Vari, R.; Veneziano, S.; Verducci, M.; Zanello, L.] INFN, Sez Roma, Rome, Italy.
[Bagiacchi, P.; Bagnaia, P.; Bauce, M.; Bini, C.; Ciapetti, G.; Di Domenico, A.; Di Donato, C.; Gauzzi, P.; Gentile, S.; Giagu, S.; Gustavino, G.; Kuna, M.; Lacava, F.; Luci, C.; Messina, A.; Monzani, S.; Vanadia, M.; Verducci, M.; Zanello, L.] Sapienza Univ Roma, Dipartimento Fis, Rome, Italy.
[Aielli, G.; Camarri, P.; Cardarelli, R.; Di Ciaccio, A.; Iuppa, R.; Liberti, B.; Salamon, A.; Santonico, R.] INFN, Sez Roma Tor Vergata, Rome, Italy.
[Aielli, G.; Camarri, P.; Di Ciaccio, A.; Iuppa, R.; Santonico, R.] Univ Roma Tor Vergata, Dipartimento Fis, Rome, Italy.
[Bacci, C.; Baroncelli, A.; Biglietti, M.; Ceradini, F.; Di Micco, B.; Farilla, A.; Graziani, E.; Iodice, M.; Orestano, D.; Pastore, F.; Petrucci, F.; Puddu, D.; Salamanna, G.; Sessa, M.; Stanescu, C.; Taccini, C.] INFN, Sez Roma Tre, Rome, Italy.
[Bacci, C.; Ceradini, F.; Di Micco, B.; Orestano, D.; Pastore, F.; Petrucci, F.; Puddu, D.; Salamanna, G.; Sessa, M.; Taccini, C.] Univ Roma Tre, Dipartimento Matemat & Fis, Rome, Italy.
[Benchekroun, D.; Chafaq, A.; Hoummada, A.] Univ Hassan 2, Fac Sci Ain Chock, Res Univ Phys Hautes Energies, Casablanca, Morocco.
[Ghazlane, H.] Ctr Natl Energie Sci Tech Nucl, Rabat, Morocco.
[El Kacimi, M.; Goujdami, D.] Univ Cadi Ayyad, Fac Sci Semlalia, LPHEA Marrakech, Marrakech, Morocco.
[Derkaoui, J. E.; Ouchrif, M.; Tayalati, Y.] Univ Mohamed Premier, Fac Sci, Oujda, Morocco.
[Derkaoui, J. E.; Ouchrif, M.; Tayalati, Y.] LPTPM, Oujda, Morocco.
[El Moursli, R. Cherkaoui; Fassi, F.; Haddad, N.; Idrissi, Z.] Univ Mohammed 5, Fac Sci, Rabat, Morocco.
[Bachacou, H.; Bauer, F.; Besson, N.; Blanchard, J. -B.; Boonekamp, M.; Calandri, A.; Chevalier, L.; Hoffmann, M. Dano; Deliot, F.; Etienvre, A. I.; Formica, A.; Giraud, P. F.; Da Costa, J. Goncalves Pinto Firmino; Guyot, C.; Hanna, R.; Hassani, S.; Kivernyk, O.; Kozanecki, W.; Kukla, R.; Lancon, E.; Laporte, J. F.; Maiani, C.; Mansoulie, B.; Meyer, J-P.; Nicolaidou, R.; Ouraou, A.; Protopapadaki, E.; Royon, C. R.; Saimpert, M.; Schoeffel, L.; Schune, Ph.; Schwemling, Ph.; Schwindling, J.] CEA Saclay Commissariat Energie Atom & Energies A, DSM IRFU Inst Rech Ies Lois Fondament Univers, Gif Sur Yvette, France.
[Battaglia, M.; Debenedetti, C.; Grabas, H. M. X.; Grillo, A. A.; Hance, M.; Kuhl, A.; LaRosa, A.; Law, A. T.; Liang, Z.; Litke, A. M.; Lockman, W. S.; Nielsen, J.; Reece, R.; Rose, P.; Sadrozinski, H. F-W.; Schumm, B. A.; Seiden, A.] Univ Calif Santa Cruz, Santa Cruz Inst Particle Phys, Santa Cruz, CA 95064 USA.
[Alpigiani, C.; Blackburn, D.; Goussiou, A. G.; Hsu, S. -C; Johnson, W. J.; Lubatti, H. J.; Marx, M.; Meehan, S.; Rompotis, N.; Rosten, R.; Rothberg, J.; Russell, H. L.; De Bruin, P. H. Sales; Pastor, E. Torro; Watts, G.] Univ Washington, Dept Phys, Seattle, WA 98195 USA.
[Anastopoulos, C.; Costanzo, D.; Donszelmann, T. Cuhadar; Dawson, I.; Fletcher, G. T.; Hamity, G. N.; Hodgkinson, M. C.; Hodgson, P.; Johansson, P.; Klinger, J. A.; Korolkova, E. V.; Kyriazopoulos, D.; Paredes, B. Lopez; Macdonald, C. M.; Miyagawa, P. S.; Paganis, E.; Parker, K. A.; Tovey, D. R.; Vickey, T.; Boeriu, O. E. Vickey] Univ Sheffield, Dept Phys & Astron, Sheffield, S Yorkshire, England.
[Hasegawa, Y.; Takeshita, T.] Shinshu Univ, Dept Phys, Nagano, Japan.
[Atlay, N. B.; Buchholz, P.; Czirr, H.; Fleck, I.; Gaur, B.; Ghasemi, S.; Ibragimov, I.; Ikematsu, K.; Rosenthal, O.; Walkowiak, W.; Ziolkowski, M.] Univ Siegen, Fachbereich Phys, Siegen, Germany.
[Buat, Q.; Horton, A. J.; Mori, D.; O'Neil, D. C.; Pachal, K.; Stelzer, B.; Temple, D.; Torres, H.; Van Nieuwkoop, J.; Vetterli, M. C.] Simon Fraser Univ, Dept Phys, Burnaby, BC, Canada.
[Barklow, T.; Bartoldus, R.; Bawa, H. S.; Black, J. E.; Cogan, J. G.; Fulsom, B. G.; Gao, Y. S.; Garelli, N.; Grenier, P.; Ilic, N.; Kagan, M.; Kocian, M.; Koi, T.; Malone, C.; Moss, J.; Mount, R.; Nachman, B. P.; Nef, P. D.; Piacquadio, G.; Rubbo, F.; Salnikov, A.; Schwartzman, A.; Strauss, E.; Su, D.; Tompkins, L.; Wittgen, M.; Young, C.; Zeng, Q.] SLAC Natl Accelerator Lab, Stanford, CA USA.
[Astalos, R.; Bartos, P.; Blazek, T.; Plazak, L.; Sykora, I.; Tokar, S.; Zenis, T.] Comenius Univ, Fac Math Phys & Informat, Bratislava, Slovakia.
[Antos, J.; Bruncko, D.; Kladiva, E.; Strizenec, P.; Urban, J.] Slovak Acad Sci, Inst Expt Phys, Dept Subnucl Phys, Kosice, Slovakia.
[Castaneda-Miranda, E.; Hamilton, A.; Lee, C. A.; Yacoob, S.] Univ Cape Town, Dept Phys, Cape Town, South Africa.
[Aurousseau, M.; Connell, S. H.; Govender, N.] Univ Johannesburg, Dept Phys, Johannesburg, South Africa.
[Hsu, C.; Kar, D.; March, L.; Garcia, B. R. Mellado; Ruan, X.] Univ Witwatersrand, Sch Phys, Johannesburg, South Africa.
[Abulaiti, Y.; Akerstedt, H.; Asman, B.; Bendtz, K.; Bertoli, G.; Bylund, O. Bessidskaia; Bohm, C.; Clement, C.; Cribbs, W. A.; Hellman, S.; Jon-And, K.; Khandanyan, H.; Klimek, P.; Lundberg, O.; Milstead, D. A.; Moa, T.; Molander, S.; Pani, P.; Plucinski, P.; Poettgen, R.; Rossetti, V.; Shcherbakova, A.; Silverstein, S. B.; Sjolin, J.; Strandberg, S.; Tylmad, M.; Ughetto, M.] Stockholm Univ, Dept Phys, Stockholm, Sweden.
[Abulaiti, Y.; Akerstedt, H.; Asman, B.; Bendtz, K.; Bertoli, G.; Bylund, O. Bessidskaia; Clement, C.; Cribbs, W. A.; Hellman, S.; Jon-And, K.; Khandanyan, H.; Klimek, P.; Lundberg, O.; Milstead, D. A.; Moa, T.; Molander, S.; Pani, P.; Plucinski, P.; Poettgen, R.; Rossetti, V.; Shcherbakova, A.; Sjolin, J.; Strandberg, S.; Tylmad, M.; Ughetto, M.] Oskar Klein Ctr, Stockholm, Sweden.
[Lund-Jensen, B.; Sidebo, P. E.; Strandberg, J.] Royal Inst Technol, Dept Phys, Stockholm, Sweden.
[Balestri, T.; Bee, C. P.; Campoverde, A.; Chen, K.; Hobbs, J.; Jia, J.; Li, H.; Lindquist, B. E.; McCarthy, R. L.; Montalbano, A.; Puldon, D.; Radhakrishnan, S. K.; Rijssenbeek, M.; Schamberger, R. D.; Tsybychev, D.; Zaman, A.; Zhou, M.] SUNY Stony Brook, Dept Phys & Astron, Stony Brook, NY 11794 USA.
[Balestri, T.; Bee, C. P.; Campoverde, A.; Chen, K.; Hobbs, J.; Jia, J.; Li, H.; Lindquist, B. E.; McCarthy, R. L.; Montalbano, A.; Puldon, D.; Radhakrishnan, S. K.; Rijssenbeek, M.; Schamberger, R. D.; Tsybychev, D.; Zaman, A.; Zhou, M.] SUNY Stony Brook, Dept Chem, Stony Brook, NY 11794 USA.
[Allbrooke, B. M. M.; Asquith, L.; Cerri, A.; Barajas, C. A. Chavez; De Sanctis, U.; De Santo, A.; Grout, Z. J.; Potter, C. J.; Salvatore, F.; Castillo, I. Santoyo; Shehu, C. Y.; Suruliz, K.; Sutton, M. R.; Vivarelli, I.] Univ Sussex, Dept Phys & Astron, Brighton, E Sussex, England.
[Black, C. W.; Cuthbert, C.; Finelli, K. D.; Jeng, G. -Y.; Limosani, A.; Morley, A. K.; Patel, N. D.; Saavedra, A. F.; Scarcella, M.; Varvell, K. E.; Wang, J.; Watson, I. J.; Yabsley, B.] Univ Sydney, Sch Phys, Sydney, NSW, Australia.
[Abdallah, J.; Hou, S.; Hsu, P. J.; Lee, S. C.; Lin, S. C.; Liu, B.; Liu, D.; Lo Sterzo, F.; Mazini, R.; Shi, L.; Soh, D. A.; Teng, P. K.; Wang, C.; Wang, S. M.; Yang, Y.] Acad Sinica, Inst Phys, Taipei, Taiwan.
[Abreu, H.; Cheatham, S.; Di Mattia, A.; Gozani, E.; Kopeliansky, R.; Musto, E.; Rozen, Y.; Tarem, S.; van Eldik, N.] Technion Israel Inst Technol, Dept Phys, Haifa, Israel.
[Abramowicz, H.; Alexander, G.; Amram, N.; Ashkenazi, A.; Bella, G.; Benary, O.; Benhammou, Y.; Davies, M.; Etzion, E.; Gershon, A.; Gueta, O.; Oren, Y.; Silver, Y.; Soffer, A.; Taiblum, N.] Tel Aviv Univ, Raymond & Beverly Sackler Sch Phys & Astron, Tel Aviv, Israel.
[Bachas, K.; Gkaitatzis, S.; Gkialas, I.; Iliadis, D.; Kimura, N.; Kordas, K.; Kourkoumeli-Charalampidi, A.; Leisos, A.; Orlando, N.; Papageorgiou, K.; Hernandez, D. Paredes; Petridou, C.; Sampsonidis, D.; Tsionou, D.] Aristotle Univ Thessaloniki, Dept Phys, Thessaloniki, Greece.
[Asai, S.; Chen, S.; Dohmae, T.; Enari, Y.; Hanawa, K.; Kanaya, N.; Kataoka, Y.; Kato, C.; Kawamoto, T.; Kazama, S.; Kobayashi, A.; Kobayashi, T.; Komori, Y.; Mashimo, T.; Masubuchi, T.; Minami, Y.; Mori, T.; Morinaga, M.; Nakamura, T.; Ninomiya, Y.; Nobe, T.; Saito, T.; Sakamoto, H.; Sasaki, Y.; Tanaka, J.; Terashi, K.; Ueda, I.; Yamamoto, S.; Yamanaka, T.] Univ Tokyo, Int Ctr Elementary Particle Phys, Tokyo, Japan.
[Asai, S.; Chen, S.; Dohmae, T.; Enari, Y.; Hanawa, K.; Kanaya, N.; Kataoka, Y.; Kato, C.; Kawamoto, T.; Kazama, S.; Kobayashi, A.; Kobayashi, T.; Komori, Y.; Mashimo, T.; Masubuchi, T.; Minami, Y.; Mori, T.; Morinaga, M.; Nakamura, T.; Ninomiya, Y.; Nobe, T.; Saito, T.; Sakamoto, H.; Sasaki, Y.; Tanaka, J.; Terashi, K.; Ueda, I.; Yamamoto, S.; Yamanaka, T.] Univ Tokyo, Dept Phys, Tokyo, Japan.
[Bratzler, U.; Fukunaga, C.] Tokyo Metropolitan Univ, Grad Sch Sci & Technol, Tokyo, Japan.
[Hirose, M.; Ishitsuka, M.; Jinnouchi, O.; Kobayashi, D.; Kuze, M.; Motohashi, K.; Nagai, R.; Pettersson, N. E.; Todome, K.; Yamaguchi, D.] Tokyo Inst Technol, Dept Phys, Tokyo, Japan.
[AbouZeid, O. S.; Batista, S. J.; Chau, C. C.; DeMarco, D. A.; Di Sipio, R.; Diamond, M.; Krieger, P.; Liblong, A.; Mc Goldrick, G.; Orr, R. S.; Polifka, R.; Rudolph, M. S.; Savard, P.; Sinervo, P.; Taenzer, J.; Teuscher, R. J.; Trischuk, W.; Veloce, L. M.; Venturi, N.] Univ Toronto, Dept Phys, Toronto, ON, Canada.
[Canepa, A.; Chekulaev, S. V.; Jovicevic, J.; Koutsman, A.; Oram, C. J.; Codina, E. Perez; Schneider, B.; Schouten, D.; Seuster, R.; Stelzer-Chilton, O.; Tafirout, R.; Trigger, I. M.] TRIUMF, Vancouver, BC, Canada.
[Garcia, J. A. Benitez; Ramos, J. Manjarres; Palacino, G.; Taylor, W.] York Univ, Dept Phys & Astron, Toronto, ON, Canada.
[Hara, K.; Hayashi, T.; Kasahara, K.; Kim, S. H.; Kiuchi, K.; Nagata, K.; Okawa, H.; Sato, K.; Ukegawa, F.] Univ Tsukuba, Fac Pure & Appl Sci, Tsukuba, Ibaraki, Japan.
[Hara, K.; Hayashi, T.; Kasahara, K.; Kim, S. H.; Kiuchi, K.; Nagata, K.; Okawa, H.; Sato, K.; Ukegawa, F.] Univ Tsukuba, Ctr Integrated Res Fundamental Sci & Engn, Tsukuba, Ibaraki, Japan.
[Beauchemin, P. H.; Meoni, E.; Sliwa, K.; Wetter, J.] Tufts Univ, Dept Phys & Astron, Medford, MA 02155 USA.
[Losada, M.; Moreno, D.; Navarro, G.; Sandoval, C.] Univ Antonio Narino, Ctr Invest, Bogota, Colombia.
[Casper, D. W.; Corso-Radu, A.; Frate, M.; Gerbaudo, D.; Guest, D.; Lankford, A. J.; Mete, A. S.; Nelson, A.; Scannicchio, D. A.; Schernau, M.; Shimmin, C. O.; Taffard, A.; Unel, G.; Whiteson, D.] Univ Calif Irvine, Dept Phys & Astron, Irvine, CA USA.
[Acharya, B. S.; Barisonzi, M.; Cobal, M.; Giordani, M. P.; Miglioranzi, S.; Pinamonti, M.; Quayle, W. B.; Serkin, L.; Shaw, K.; Soualah, R.; Truong, L.] INFN, Sez Trieste, Grp Collegato Udine, Udine, Italy.
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[Cobal, M.; Giordani, M. P.; Miglioranzi, S.; Pinamonti, M.; Soualah, R.; Truong, L.] Univ Udine, Dipartimento Chim Fis & Ambiente, Udine, Italy.
[Atkinson, M.; Basye, A.; Armadans, R. Caminal; Cavaliere, V.; Chang, P.; Errede, S.; Lie, K.; Liss, T. M.; Liu, L.; Long, J. D.; Neubauer, M. S.; Rybar, M.; Shang, R.; Vichou, I.; Zeng, J. C.] Univ Illinois, Dept Phys, 1110 W Green St, Urbana, IL 61801 USA.
[Kuutmann, E. Bergeaas; Brenner, R.; Ekelof, T.; Ellert, M.; Ferrari, A.; Gradin, P. O. J.; Isaksson, C.; Ohman, H.; Pelikan, D.; Rangel-Smith, C.] Uppsala Univ, Dept Phys & Astron, Uppsala, Sweden.
[Ferrer, A.; Fiorini, L.; Fuster, J.; Garcia, C.; Navarro, J. E. Garcia; Higon-Rodriguez, E.; Quiles, A. Irles; Pena, J. Jimenez; Kaci, M.; King, M.; Lacasta, C.; Garcia-Estan, M. T. Perez; Salt, J.; Sanchez, J.; Valero, A.; Ferrer, J. A. Valls; Vos, M.] Univ Valencia, Inst Fis Corpuscular IFIC, Valencia, Spain.
[Piqueras, D. Alvarez; Urban, S. Cabrera; Gimenez, V. Castillo; Alberich, L. Cerda; Costa, M. J.; Martinez, P. Fernandez; Ferrer, A.; Fiorini, L.; Fuster, J.; Garcia, C.; Navarro, J. E. Garcia; de la Hoz, S. Gonzalez; Jimenez, Y. Hernandez; Higon-Rodriguez, E.; Quiles, A. Irles; Pena, J. Jimenez; Kaci, M.; King, M.; Lacasta, C.; Lacuesta, V. R.; Marti-Garcia, S.; Mitsou, V. A.; Lopez, S. Pedraza; Garcia-Estan, M. T. Perez; Adam, E. Romero; Ros, E.; Salt, J.; Sanchez, J.; Martinez, V. Sanchez; Soldevila, U.; Valero, A.; Ferrer, J. A. Valls; Vos, M.] Univ Valencia, Dept Fis Atom Mol & Nucl, Valencia, Spain.
[Piqueras, D. Alvarez; Urban, S. Cabrera; Gimenez, V. Castillo; Alberich, L. Cerda; Costa, M. J.; Martinez, P. Fernandez; Ferrer, A.; Fiorini, L.; Fuster, J.; Garcia, C.; Navarro, J. E. Garcia; de la Hoz, S. Gonzalez; Jimenez, Y. Hernandez; Higon-Rodriguez, E.; Quiles, A. Irles; Pena, J. Jimenez; Kaci, M.; King, M.; Lacasta, C.; Lacuesta, V. R.; Marti-Garcia, S.; Mitsou, V. A.; Lopez, S. Pedraza; Garcia-Estan, M. T. Perez; Adam, E. Romero; Ros, E.; Salt, J.; Sanchez, J.; Martinez, V. Sanchez; Soldevila, U.; Valero, A.; Ferrer, J. A. Valls; Vos, M.] Univ Valencia, Dept Ingn Elect, Valencia, Spain.
[Piqueras, D. Alvarez; Urban, S. Cabrera; Gimenez, V. Castillo; Alberich, L. Cerda; Costa, M. J.; Martinez, P. Fernandez; Ferrer, A.; Fiorini, L.; Fuster, J.; Garcia, C.; Navarro, J. E. Garcia; de la Hoz, S. Gonzalez; Jimenez, Y. Hernandez; Higon-Rodriguez, E.; Quiles, A. Irles; Pena, J. Jimenez; Kaci, M.; King, M.; Lacasta, C.; Lacuesta, V. R.; Marti-Garcia, S.; Mitsou, V. A.; Lopez, S. Pedraza; Garcia-Estan, M. T. Perez; Adam, E. Romero; Ros, E.; Salt, J.; Sanchez, J.; Martinez, V. Sanchez; Soldevila, U.; Valero, A.; Ferrer, J. A. Valls; Vos, M.] Univ Valencia, IMB CNM, Valencia, Spain.
[Piqueras, D. Alvarez; Urban, S. Cabrera; Gimenez, V. Castillo; Alberich, L. Cerda; Costa, M. J.; Martinez, P. Fernandez; Ferrer, A.; Fiorini, L.; Fuster, J.; Garcia, C.; Navarro, J. E. Garcia; de la Hoz, S. Gonzalez; Jimenez, Y. Hernandez; Higon-Rodriguez, E.; Quiles, A. Irles; Pena, J. Jimenez; Kaci, M.; King, M.; Lacasta, C.; Lacuesta, V. R.; Marti-Garcia, S.; Mitsou, V. A.; Lopez, S. Pedraza; Garcia-Estan, M. T. Perez; Adam, E. Romero; Ros, E.; Salt, J.; Sanchez, J.; Martinez, V. Sanchez; Soldevila, U.; Valero, A.; Ferrer, J. A. Valls; Vos, M.] CSIC, Valencia, Spain.
[Danninger, M.; Fedorko, W.; Gay, C.; Gecse, Z.; Gignac, M.; Henkelmann, S.; King, S. B.; Lister, A.] Univ British Columbia, Dept Phys, Vancouver, BC, Canada.
[Albert, J.; Berghaus, F.; David, C.; Elliot, A. A.; Fincke-Keeler, M.; Hamano, K.; Hill, E.; Keeler, R.; Kowalewski, R.; Kuwertz, E. S.; Kwan, T.; LeBlanc, M.; Lefebvre, M.; Marino, C. P.; McPherson, R. A.; Pearce, J.; Sobie, R.; Trovatelli, M.; Venturi, M.] Univ Victoria, Dept Phys & Astron, Victoria, BC, Canada.
[Beckingham, M.; Farrington, S. M.; Harrison, P. F.; Jeske, C.; Jones, G.; Martin, T. A.; Murray, W. J.; Pianori, E.; Spangenberg, M.] Univ Warwick, Dept Phys, Coventry, W Midlands, England.
[Iizawa, T.; Mitani, T.; Sakurai, Y.; Yorita, K.] Waseda Univ, Tokyo, Japan.
[Bressler, S.; Citron, Z. H.; Duchovni, E.; Gross, E.; Lellouch, D.; Levinson, L. J.; Mikenberg, G.; Pitt, M.; Roth, I.; Schaarschmidt, J.; Smakhtin, V.] Weizmann Inst Sci, Dept Particle Phys, Rehovot, Israel.
[Banerjee, Sw.; Hard, A. S.; Heng, Y.; Ji, H.; Ju, X.; Kaplan, L. S.; Kashif, L.; Kruse, A.; Ming, Y.; Pan, Y. B.; Wang, F.; Wiedenmann, W.; Wu, S. L.; Yang, H.; Zhang, F.; Zobernig, G.] Univ Wisconsin, Dept Phys, Madison, WI USA.
[Kuger, F.; Redelbach, A.; Schreyer, M.; Sidiropoulou, O.; Siragusa, G.; Strohmer, R.; Tam, J. Y. C.; Trefzger, T.; Weber, S. W.; Zibell, A.] Julius Maximilians Univ, Fak Phys & Astron, Wurzburg, Germany.
[Bannoura, A. A. E.; Braun, H. M.; Cornelissen, T.; Ellinghaus, F.; Ernis, G.; Fischer, J.; Flick, T.; Gabizon, O.; Hamacher, K.; Harenberg, T.; Heim, T.; Hirschbuehl, D.; Kersten, S.; Kohlmann, S.; Mattig, P.; Neumann, M.; Pataraia, S.; Riegel, C. J.; Sandhoff, M.; Tepel, F.; Wagner, W.; Zeitnitz, C.] Berg Univ Wuppertal, Fachbereich Phys C, Wuppertal, Germany.
[Baker, O. K.; Cummings, J.; Demers, S.; Garberson, F.; Henrichs, A.; Ideal, E.; Lagouri, T.; Leister, A. G.; Loginov, A.; Milov, A.; Thomsen, L. A.; Tipton, P.; Wang, X.] Yale Univ, Dept Phys, New Haven, CT USA.
[Hakobyan, H.; Vardanyan, G.] Yerevan Phys Inst, Yerevan, Armenia.
[Rahal, G.] IN2P3, Ctr Calcul, Villeurbanne, France.
[Acharya, B. S.] Kings Coll London, Dept Phys, London, England.
[Ahmadov, F.; Huseynov, N.; Javadov, N.] Azerbaijan Acad Sci, Inst Phys, Baku, Azerbaijan.
[Anisenkov, A. V.; Baldin, E. M.; Bobrovnikov, V. S.; Buzykaev, A. R.; Kazanin, V. F.; Kharlamov, A. G.; Korol, A. A.; Maslennikov, A. L.; Maximov, D. A.; Peleganchuk, S. V.; Rezanova, O. L.; Soukharev, A. M.; Talyshev, A. A.; Tikhonov, Yu. A.] Novosibirsk State Univ, Novosibirsk, Russia.
[Azuelos, G.; Gingrich, D. M.; Oakham, F. G.; Savard, P.; Vetterli, M. C.] TRIUMF, Vancouver, BC, Canada.
[Banerjee, Sw.] Univ Louisville, Dept Phys & Astron, Louisville, KY 40292 USA.
[Bawa, H. S.; Gao, Y. S.] Calif State Univ Fresno, Dept Phys, Fresno, CA 93740 USA.
[Beck, H. P.] Univ Fribourg, Dept Phys, Fribourg, Switzerland.
[Castro, N. F.] Univ Autonoma Barcelona, Dept Fis, Barcelona, Spain.
[Chelkov, G. A.] Univ Porto, Dept Fis & Astron, Fac Ciencias, Oporto, Portugal.
[Chen, L.; Zhang, R.] Tomsk State Univ, Tomsk, Russia.
[Conventi, F.; Della Pietra, M.] Univ Napoli Parthenope, Naples, Italy.
[Corriveau, F.; McPherson, R. A.; Robertson, S. H.; Sobie, R.; Teuscher, R. J.] Inst Particle Phys IPP, Wuhan, Peoples R China.
[Davies, E.] Natl Inst Phys & Nucl Engn, Bucharest, Romania.
[Fedin, O. L.] St Petersburg State Polytech Univ, Dept Phys, St Petersburg, Russia.
[Geng, C.; Guo, Y.] Univ Michigan, Dept Phys, Ann Arbor, MI 48109 USA.
[Greenwood, Z. D.; Sawyer, L.] Ctr High Performance Comp, CSIR Campus, Cape Town, South Africa.
[Grinstein, S.; Rozas, A. Juste; Martinez, M.] Louisiana Tech Univ, Ruston, LA 71270 USA.
[Hanagaki, K.] ICREA, Barcelona, Spain.
[Hsu, P. J.] Osaka Univ, Grad Sch Sci, Osaka, Japan.
[Ilchenko, Y.; Onyisi, P. U. E.] Natl Tsing Hua Univ, Dept Phys, Hsinchu, Taiwan.
[Jejelava, J.] Radboud Univ Nijmegen, Nikhef, Inst Math Astrophys & Particle Phys, Nijmegen, Netherlands.
[Jenni, P.] Univ Texas Austin, Dept Phys, Austin, TX 78712 USA.
[Khubua, J.] Ilia State Univ, Inst Theoret Phys, Tbilisi, Rep of Georgia.
[Konoplich, R.] CERN, Geneva, Switzerland.
[Leisos, A.] GTU, Tbilisi, Rep of Georgia.
[Li, B.; Song, H. Y.] Ochanomizu Univ, Ochadai Acad Prod, Tokyo, Japan.
[Li, Y.] Manhattan Coll, New York, NY USA.
Hellen Open Univ, Patras, Greece.
[Liu, B.] Acad Sinica, Acad Sinica Grid Comp, Inst Phys, Taipei, Taiwan.
[Myagkov, A. G.; Nikolaenko, V.; Zaitsev, A. M.] Shandong Univ, Sch Phys, Jinan, Shandong, Peoples R China.
[Nessi, M.] Moscow Inst Phys & Technol, Dolgoprudnyi, Russia.
[Pinamonti, M.] Univ Geneva, Sect Phys, Geneva, Switzerland.
[Purohit, M.] Eotvos Lorand Univ, Budapest, Hungary.
[Shi, L.; Soh, D. A.] Int Sch Adv Studies SISSA, Trieste, Italy.
[Smirnova, L. N.; Turchikhin, S.] Univ South Carolina, Dept Phys & Astron, Columbia, SC USA.
[Tikhomirov, V. O.] Sun Yat Sen Univ, Sch Phys & Engn, Guangzhou, Guangdong, Peoples R China.
[Tompkins, L.] Bulgarian Acad Sci, Inst Nucl Res & Nucl Energy INRNE, Sofia, Bulgaria.
[Toth, J.] Moscow MV Lomonosov State Univ, Fac Phys, Moscow, Russia.
[Yusuff, I.] Acad Sinica, Inst Phys, Taipei, Taiwan.
Natl Res Nucl Univ MEPhI, Moscow, Russia.
Stanford Univ, Dept Phys, Stanford, CA 94305 USA.
Wigner Res Ctr Phys, Inst Particle & Nucl Phys, Budapest, Hungary.
Flensburg Univ Appl Sci, Flensburg, Germany.
Univ Malaya, Dept Phys, Kuala Lumpur, Malaysia.
Aix Marseille Univ, CPPM, Marseille, France.
CNRS, IN2P3, Marseille, France.
RP Aad, G (reprint author), MAix Marseille Univ, CPP, Marseille, France.; Aad, G (reprint author), CNRS, IN2P3, Marseille, France.
RI Chekulaev, Sergey/O-1145-2015; Gladilin, Leonid/B-5226-2011; Solodkov,
Alexander/B-8623-2017; Tikhomirov, Vladimir/M-6194-2015; Doyle,
Anthony/C-5889-2009; Zaitsev, Alexandre/B-8989-2017; Leitner,
Rupert/C-2004-2017; Carli, Ina/C-2189-2017; messina, andrea/C-2753-2013;
Guo, Jun/O-5202-2015; Livan, Michele/D-7531-2012; Villa,
Mauro/C-9883-2009; Peleganchuk, Sergey/J-6722-2014; Yang,
Haijun/O-1055-2015; Li, Liang/O-1107-2015; Monzani, Simone/D-6328-2017;
Warburton, Andreas/N-8028-2013; Kuday, Sinan/C-8528-2014; Mitsou,
Vasiliki/D-1967-2009; Camarri, Paolo/M-7979-2015; Carvalho,
Joao/M-4060-2013; Prokoshin, Fedor/E-2795-2012
OI Gladilin, Leonid/0000-0001-9422-8636; Solodkov,
Alexander/0000-0002-2737-8674; Tikhomirov, Vladimir/0000-0002-9634-0581;
Doyle, Anthony/0000-0001-6322-6195; Zaitsev,
Alexandre/0000-0002-4961-8368; Leitner, Rupert/0000-0002-2994-2187;
Carli, Ina/0000-0002-0411-1141; Guo, Jun/0000-0001-8125-9433; Livan,
Michele/0000-0002-5877-0062; Villa, Mauro/0000-0002-9181-8048;
Peleganchuk, Sergey/0000-0003-0907-7592; Li, Liang/0000-0001-6411-6107;
Monzani, Simone/0000-0002-0479-2207; Warburton,
Andreas/0000-0002-2298-7315; Kuday, Sinan/0000-0002-0116-5494; Mitsou,
Vasiliki/0000-0002-1533-8886; Camarri, Paolo/0000-0002-5732-5645;
Carvalho, Joao/0000-0002-3015-7821; Prokoshin, Fedor/0000-0001-6389-5399
FU ANPCyT, Argentina; YerPhI, Armenia; ARC, Australia; BMWF, Austria; FWF,
Austria; ANAS, Azerbaijan; SSTC, Belarus; CNPq, Brazil; FAPESP, Brazil;
NSERC, Canada; NRC, Canada; CFI, Canada; CERN; CONICYT, Chile; CAS,
China; MOST, China; NSFC, China; COLCIEN-CIAS, Colombia; MSMT CR, Czech
Republic; MPO CR, Czech Republic; VSC CR, Czech Republic; DNRF, Denmark;
DNSRC, Denmark; Lundbeck Foundation, Denmark; EPLANET; ERC; NSRF;
European Union; IN2P3-CNRS, France; CEA-DSM/IRFU, France; GNSF, Georgia;
BMBF, Germany; DFG, Germany; HGF, Germany; MPG, Germany; AvH Foundation,
Germany; GSRT, Greece; NSRF, Greece; ISF, Israel; MINERVA, Israel; GIF,
Israel; DIP, Israel; Benoziyo Center, Israel; INFN, Italy; MEXT, Japan;
JSPS, Japan; CNRST, Morocco; FOM, Netherlands; NWO, Netherlands; BRF,
Norway; RCN, Norway; MNiSW, Poland; GRICES, Portugal; FCT, Portugal;
MERYS (MECTS), Romania; MES of Russia; ROSATOM, Russian Federation;
JINR; MSTD, Serbia; MSSR, Slovakia; ARRS, Slovenia; MIZS, Slovenia;
DST/NRF, South Africa; MICINN, Spain; SRC, Sweden; Wallenberg
Foundation, Sweden; SER, Switzerland; SNSF, Switzerland; Canton of Bern,
Switzerland; Canton of Geneva, Switzerland; NSC, Taiwan; TAEK, Turkey;
STFC, United Kingdom; Royal Society, United Kingdom; Leverhulme Trust,
United Kingdom; DOE, United States of America; NSF, United States of
America
FX We thank CERN for the very successful operation of the LHC, as well as
the support staff from our institutions without whom ATLAS could not be
operated efficiently. We acknowledge the support of ANPCyT, Argentina;
YerPhI, Armenia; ARC, Australia; BMWF and FWF, Austria; ANAS,
Azerbaijan; SSTC, Belarus; CNPq and FAPESP, Brazil; NSERC, NRC and CFI,
Canada; CERN; CONICYT, Chile; CAS, MOST and NSFC, China; COLCIEN-CIAS,
Colombia; MSMT CR, MPO CR and VSC CR, Czech Republic; DNRF, DNSRC and
Lundbeck Foundation, Denmark; EPLANET, ERC and NSRF, European Union;
IN2P3-CNRS, CEA-DSM/IRFU, France; GNSF, Georgia; BMBF, DFG, HGF, MPG and
AvH Foundation, Germany; GSRT and NSRF, Greece; ISF, MINERVA, GIF, DIP
and Benoziyo Center, Israel; INFN, Italy; MEXT and JSPS, Japan; CNRST,
Morocco; FOM and NWO, Netherlands; BRF and RCN, Norway; MNiSW, Poland;
GRICES and FCT, Portugal; MERYS (MECTS), Romania; MES of Russia and
ROSATOM, Russian Federation; JINR; MSTD, Serbia; MSSR, Slovakia; ARRS
and MIZS, Slovenia; DST/NRF, South Africa; MICINN, Spain; SRC and
Wallenberg Foundation, Sweden; SER, SNSF and Cantons of Bern and Geneva,
Switzerland; NSC, Taiwan; TAEK, Turkey; STFC, the Royal Society and
Leverhulme Trust, United Kingdom; DOE and NSF, United States of America.
The crucial computing support from all WLCG partners is acknowledged
gratefully, in particular from CERN and the ATLAS Tier-1 facilities at
TRIUMF (Canada), NDGF (Denmark, Norway, Sweden), CC-IN2P3 (France),
KIT/GridKA (Germany), INFN-CNAF (Italy), NL-T1 (Netherlands), PIC
(Spain), ASGC (Taiwan), RAL (UK) and BNL (USA) and in the Tier-2
facilities worldwide.
NR 81
TC 0
Z9 0
U1 30
U2 30
PU SPRINGER
PI NEW YORK
PA 233 SPRING ST, NEW YORK, NY 10013 USA
SN 1434-6044
EI 1434-6052
J9 EUR PHYS J C
JI Eur. Phys. J. C
PD OCT 3
PY 2016
VL 76
IS 10
AR 538
DI 10.1140/epjc/s10052-016-4366-4
PG 39
WC Physics, Particles & Fields
SC Physics
GA DY5UB
UT WOS:000385168100001
ER
PT J
AU Monroe, AP
Chandler, RB
Burger, LW
Martin, JA
AF Monroe, Adrian P.
Chandler, Richard B.
Burger, L. Wes, Jr.
Martin, James A.
TI Converting exotic forages to native warm-season grass can increase avian
productivity in beef production systems
SO AGRICULTURE ECOSYSTEMS & ENVIRONMENT
LA English
DT Article
DE Bayesian analysis; Detection error; Dickcissel; Land-sharing; Native
warm-season grasses; Spiza americana
ID DICKCISSELS SPIZA-AMERICANA; CONSERVATION RESERVE PROGRAM; TALLGRASS
PRAIRIE; NEST PREDATION; HABITAT QUALITY; WILDLIFE HABITAT; AREA
SENSITIVITY; UNITED-STATES; BIRDS; SURVIVAL
AB Grasslands are among the most imperiled ecosystems in the world, and establishment of exotic forage grasses and management for uniform utilization may have contributed to population declines of many obligate grassland bird species in North America. Native warm-season grasses (NWSG) are increasingly promoted as viable alternatives to exotic forages currently in production such as bermudagrass (Cynodon dactylon) and tall fescue (Schedonorus arundinaceus), but structure of native bunchgrasses also may offer nesting habitat for birds such as the dickcissel (Spiza americana). Establishing NWSG pastures may thereby create an opportunity for land-sharing, where agriculture incorporates biodiversity-friendly practices. We investigated diciccissel responses to NWSG and grazing at the Prairie Research Unit in Monroe Co., Mississippi (USA), where we established a gradient of management intensity among four treatments in small, operational-scale pastures (6.4-10.5 ha). Treatments included grazed exotic forages, two grazed NWSG treatments including Indian grass (Sorghastrum nutans) monoculture and grazed mixed NWSG polyculture of Indian grass, little bluestem (Schizachyrium scoparium), and big bluestem (Andropogon gerardii), and a non-grazed NWSG polyculture treatment. We applied a multi-state capture recapture model in a Bayesian framework to estimate dickcissel nest density and productivity while accounting for nest stage-specific variation in survival and detection. Nest density and productivity were consistently greater in non-grazed NWSG than grazed exotic pasture, whereas productivity in grazed NWSG treatments was intermediate but declined between years. We also found that variation in survival and density did not always correspond with estimated productivity, and thus solely relying on either parameter may be misleading when making inferences on habitat quality. These results suggest a positive response to NWSG among dickcissels in this system, but grazing may reduce nest site abundance, and consequently productivity. Native warm-season forages may be a viable land-sharing alternative by increasing productivity of tall structure specialists such as dickcissels compared with exotic grass pastures currently in production, but grazing should be managed to ensure abundance of tall vegetation structure for nest sites. (C) 2016 Elsevier B.V. All rights reserved.
C1 [Monroe, Adrian P.; Burger, L. Wes, Jr.; Martin, James A.] Mississippi State Univ, Dept Wildlife Fisheries & Aquaculture, Mississippi State, MS 39762 USA.
[Chandler, Richard B.] Univ Georgia, Warnell Sch Forestry & Nat Resources, Athens, GA 30602 USA.
[Monroe, Adrian P.] Colorado State Univ, Nat Resource Ecol Lab, Dept 1499, Ft Collins, CO 80523 USA.
[Martin, James A.] Univ Georgia, Warnell Sch Forestry & Nat Resources, Savannah River Ecol Lab, Athens, GA 30602 USA.
RP Monroe, AP (reprint author), Mississippi State Univ, Dept Wildlife Fisheries & Aquaculture, Mississippi State, MS 39762 USA.; Monroe, AP (reprint author), Colorado State Univ, Nat Resource Ecol Lab, Dept 1499, Ft Collins, CO 80523 USA.
EM apmonr@gmail.com; rchandler@warnell.uga.edu; lwb6@msstate.edu;
martinj@warnell.uga.edu
OI Monroe, Adrian/0000-0003-0934-8225
FU USDA NRCS Agricultural Wildlife Conservation Center; Mississippi
Agricultural and Forestry Experiment Station (MAFES); Southern
Sustainable Agriculture Research & Education (SARE) graduate student
grant; Forest and Wildlife Research Center at Mississippi State
University; College of Forest Resources at Mississippi State University;
National Institute of Food and Agriculture, U.S. Department of
Agriculture [206903]
FX We are indebted to our friend and colleague Sam Riffell for his
conceptual and financial support of the larger grazing and bird study.
We are also grateful to W. Batton, C. Bogan, J. Burger, A. Clark, K.
Drey, S. Easley, K. Fleming, T. Guthrie, L. Latino, M. McConnell, B.
McKinley, E. O'Donnell, M. Thornton, and A. Tisdale for their assistance
with nest-searching and monitoring. K. Evans, K. Newcomb, and S. Riffell
offered helpful comments that improved earlier versions of this
manuscript. R. Conover provided guidance on ageing dickcissel eggs and
nestlings. H. Boland, T. Best, and the Mississippi State University
Prairie Research Unit managed livestock for our study. Funding was
provided by the USDA NRCS Agricultural Wildlife Conservation Center, the
Mississippi Agricultural and Forestry Experiment Station (MAFES), and a
Southern Sustainable Agriculture Research & Education (SARE) graduate
student grant. The Forest and Wildlife Research Center and College of
Forest Resources at Mississippi State University provided additional
support. This material is based upon work that was supported by the
National Institute of Food and Agriculture, U.S. Department of
Agriculture, Hatch project under accession number 206903.
NR 96
TC 0
Z9 0
U1 3
U2 3
PU ELSEVIER SCIENCE BV
PI AMSTERDAM
PA PO BOX 211, 1000 AE AMSTERDAM, NETHERLANDS
SN 0167-8809
EI 1873-2305
J9 AGR ECOSYST ENVIRON
JI Agric. Ecosyst. Environ.
PD OCT 3
PY 2016
VL 233
BP 85
EP 93
DI 10.1016/j.agee.2016.08.024
PG 9
WC Agriculture, Multidisciplinary; Ecology; Environmental Sciences
SC Agriculture; Environmental Sciences & Ecology
GA ED7YK
UT WOS:000389088400010
ER
PT J
AU Oates, LG
Duncan, DS
Sanford, GR
Liang, C
Jackson, RD
AF Oates, Lawrence G.
Duncan, David S.
Sanford, Gregg R.
Liang, Chao
Jackson, Randall D.
TI Bioenergy cropping systems that incorporate native grasses stimulate
growth of plant\-associated soil microbes in the absence of nitrogen
fertilization
SO AGRICULTURE ECOSYSTEMS & ENVIRONMENT
LA English
DT Article
DE AM fungi; Gram-negative bacteria; Cellulosic biomass; Phospholipid fatty
acid; Perennial agroecosystems; Plant-microbe interactions
ID SIGNATURE FATTY-ACIDS; CARBON SEQUESTRATION; COMMUNITY STRUCTURE;
MYCORRHIZAL FUNGI; LIPID ANALYSIS; LAND-USE; BIOMASS; PRODUCTIVITY;
RHIZOSPHERE; ABUNDANCE
AB The choice of crops and their management can strongly influence soil microbial communities and their processes. We used lipid biomarker profiling to characterize how soil microbial composition of five potential bioenergy cropping systems diverged from a common baseline five years after they were established. The cropping systems we studied included an annual system (continuous no-till corn) and four perennial crops (switchgrass, miscanthus, hybrid poplar, and restored prairie). Partial- and no-stover removal were compared for the corn system, while N-additions were compared to unfertilized plots for the perennial cropping systems. Arbuscular mycorrhizal fungi (AMF) and Gram-negative biomass was higher in unfertilized perennial grass systems, especially in switchgrass and prairie. Gram-positive bacterial biomass decreased in all systems relative to baseline values in surface soils (0-10 cm), but not subsurface soils (10-25 cm). Overall microbial composition was similar between the two soil depths. Our findings demonstrate the capacity of unfertilized perennial cropping systems to recreate microbial composition found in undisturbed soil environments and indicate how strongly agroecosystem management decisions such as N addition and plant community composition can influence soil microbial assemblages. (C) 2016 The Author(s). Published by Elsevier B.V.
C1 [Oates, Lawrence G.; Duncan, David S.; Sanford, Gregg R.; Liang, Chao; Jackson, Randall D.] Univ Wisconsin, US DOE, Great Lakes Bioenergy Res Ctr, Madison, WI 53726 USA.
[Oates, Lawrence G.; Duncan, David S.; Sanford, Gregg R.; Jackson, Randall D.] Univ Wisconsin, Dept Agron, Madison, WI 53706 USA.
[Liang, Chao] Chinese Acad Sci, Inst Appl Ecol, Shenyang 110016, Peoples R China.
RP Oates, LG (reprint author), Univ Wisconsin, US DOE, Great Lakes Bioenergy Res Ctr, Madison, WI 53726 USA.
EM oates@wisc.edu
OI Oates, Lawrence/0000-0003-4829-7600
FU DOE-Great Lakes Bioenergy Research Center (DOE BER Office of Science)
[DE-FC02-07ER64494]; DOE OBP Office of Energy Efficiency and Renewable
Energy [DE-AC05-76RL01830]
FX We thank J. Tesmer, J. Sustachek, A. Miller, Z. Andersen, B. Faust, L.
Lipps, J. Hall, and S. Miramontes for assistance in the field sampling
and laboratory prep, and H. Read and D. Williams for assistance with
extraction and identification of lipid biomarkers. Funding was provided
by the DOE-Great Lakes Bioenergy Research Center (DOE BER Office of
Science DE-FC02-07ER64494) and the DOE OBP Office of Energy Efficiency
and Renewable Energy (DE-AC05-76RL01830).
NR 61
TC 0
Z9 0
U1 14
U2 14
PU ELSEVIER SCIENCE BV
PI AMSTERDAM
PA PO BOX 211, 1000 AE AMSTERDAM, NETHERLANDS
SN 0167-8809
EI 1873-2305
J9 AGR ECOSYST ENVIRON
JI Agric. Ecosyst. Environ.
PD OCT 3
PY 2016
VL 233
BP 396
EP 403
DI 10.1016/j.agee.2016.09.008
PG 8
WC Agriculture, Multidisciplinary; Ecology; Environmental Sciences
SC Agriculture; Environmental Sciences & Ecology
GA ED7YK
UT WOS:000389088400042
ER
PT J
AU Alaee, R
Kadic, M
Rockstuhl, C
Passian, A
AF Alaee, Rasoul
Kadic, Muamer
Rockstuhl, Carsten
Passian, Ali
TI Optically assisted trapping with high-permittivity dielectric rings:
Towards optical aerosol filtration
SO APPLIED PHYSICS LETTERS
LA English
DT Article
ID PARTICLES; FORCES; MICROCANTILEVERS; NANOPARTICLES; SCATTERING; BEAM
AB Controlling the transport, trapping, and filtering of nanoparticles is important for many applications. By virtue of their weak response to gravity and their thermal motion, various physical mechanisms can be exploited for such operations on nanoparticles. However, the manipulation based on optical forces is potentially most appealing since it constitutes a highly deterministic approach. Plasmonic nanostructures have been suggested for this purpose, but they possess the disadvantages of locally generating heat and trapping the nanoparticles directly on the surface. Here, we propose the use of dielectric rings made of high permittivity materials for trapping nanoparticles. Thanks to their ability to strongly localize the field in space, nanoparticles can be trapped without contact. We use a semi-analytical method to study the ability of these rings to trap nanoparticles. The results are supported by full-wave simulations. Application of the trapping concept to nanoparticle filtration is suggested. Published by AIP Publishing.
C1 [Alaee, Rasoul; Rockstuhl, Carsten] Karlsruhe Inst Technol, Inst Theoret Solid State Phys, D-76131 Karlsruhe, Germany.
[Alaee, Rasoul] Max Planck Inst Sci Light, D-91058 Erlangen, Germany.
[Kadic, Muamer] Karlsruhe Inst Technol, Inst Appl Phys, D-76128 Karlsruhe, Germany.
[Kadic, Muamer] Univ Bourgogne Franche Comte, Inst FEMTO ST, CNRS, F-25044 Besancon, France.
[Rockstuhl, Carsten] Karlsruhe Inst Technol, Inst Nanotechnol, D-76021 Karlsruhe, Germany.
[Passian, Ali] Oak Ridge Natl Lab, Computat Sci & Engn Div, Oak Ridge, TN 37831 USA.
[Passian, Ali] Univ Tennessee, Dept Phys & Astron, Knoxville, TN 37996 USA.
RP Alaee, R (reprint author), Karlsruhe Inst Technol, Inst Theoret Solid State Phys, D-76131 Karlsruhe, Germany.; Alaee, R (reprint author), Max Planck Inst Sci Light, D-91058 Erlangen, Germany.
RI Rockstuhl, Carsten/S-5832-2016
FU Deutsche Forschungsgemeinschaft [CRC 1173]; U. S. DOE
[DE-AC05-00OR22725]; laboratory directed research and development fund
at Oak Ridge National Laboratory (ORNL); Hector Fellow Academy
FX This research was supported in part by the laboratory directed research
and development fund at Oak Ridge National Laboratory (ORNL). M.K.
acknowledges support from Hector Fellow Academy. R.A. and C.R.
acknowledge partial financial support by the Deutsche
Forschungsgemeinschaft through CRC 1173. ORNL is managed by UT-Battelle,
LLC, for the U. S. DOE under Contract No. DE-AC05-00OR22725.
NR 34
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U2 2
PU AMER INST PHYSICS
PI MELVILLE
PA 1305 WALT WHITMAN RD, STE 300, MELVILLE, NY 11747-4501 USA
SN 0003-6951
EI 1077-3118
J9 APPL PHYS LETT
JI Appl. Phys. Lett.
PD OCT 3
PY 2016
VL 109
IS 14
AR 141102
DI 10.1063/1.4963862
PG 5
WC Physics, Applied
SC Physics
GA DZ8WJ
UT WOS:000386152800002
ER
PT J
AU Antipov, S
Baryshev, SV
Kostin, R
Baturin, S
Qiu, J
Jing, C
Swinson, C
Fedurin, M
Wang, D
AF Antipov, S.
Baryshev, S. V.
Kostin, R.
Baturin, S.
Qiu, J.
Jing, C.
Swinson, C.
Fedurin, M.
Wang, D.
TI Efficient extraction of high power THz radiation generated by an
ultra-relativistic electron beam in a dielectric loaded waveguide
SO APPLIED PHYSICS LETTERS
LA English
DT Article
ID LASER; OPERATION
AB We have measured an intense THz radiation produced by a sub-picosecond, relativistic electron bunch in a dielectric loaded waveguide. For efficient THz pulse extraction, the dielectric loaded waveguide end was cut at an angle. For an appropriate choice of angle cut, such antenna converts the TM01 mode excited in the waveguide into a free-space fundamental Gauss-Hermite mode propagating at an angle with respect to the electron beam trajectory. Simulations show that more than 95% of energy can be extracted using such a simple approach. More than 40 oscillations of about 170 ps long 0.48 THz signal were explicitly measured with an interferometer and 10 mu J of energy per pulse, as determined with a calorimetric energy meter, were delivered outside the electron beamline to an area suitable for THz experiments. Published by AIP Publishing.
C1 [Antipov, S.; Baryshev, S. V.; Kostin, R.; Baturin, S.; Qiu, J.; Jing, C.] Euclid Techlabs LLC, Solon, OH 44139 USA.
[Swinson, C.; Fedurin, M.] Brookhaven Natl Lab, Accelerator Test Facil, Upton, NY 11973 USA.
[Wang, D.] Argonne Natl Lab, Argonne Wakefield Accelerator Facil, 9700 S Cass Ave, Argonne, IL 60439 USA.
[Wang, D.] Tsinghua Univ, Beijing 100084, Peoples R China.
RP Antipov, S (reprint author), Euclid Techlabs LLC, Solon, OH 44139 USA.
EM s.antipov@euclidtechlabs.com
FU DOE SBIR program [DE-SC0009571]
FX We are indebted to A. Zholents, P. Schoessow, and A. Kanareykin for
helpful discussions on the topic of wakefield generation. Accelerator
Test Facility staff are acknowledged for technical support. Euclid
Techlabs LLC acknowledges support from the DOE SBIR program Grant No.
DE-SC0009571.
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PI MELVILLE
PA 1305 WALT WHITMAN RD, STE 300, MELVILLE, NY 11747-4501 USA
SN 0003-6951
EI 1077-3118
J9 APPL PHYS LETT
JI Appl. Phys. Lett.
PD OCT 3
PY 2016
VL 109
IS 14
AR 142901
DI 10.1063/1.4963762
PG 4
WC Physics, Applied
SC Physics
GA DZ8WJ
UT WOS:000386152800037
ER
PT J
AU Enriquez, E
Chen, AP
Harrell, Z
Lu, XJ
Dowden, P
Koskelo, N
Janoschek, M
Chen, CL
Jia, QX
AF Enriquez, Erik
Chen, Aiping
Harrell, Zach
Lu, Xujie
Dowden, Paul
Koskelo, Nicholas
Janoschek, Marc
Chen, Chonglin
Jia, Quanxi
TI Oxygen vacancy-driven evolution of structural and electrical properties
in SrFeO3-delta thin films and a method of stabilization
SO APPLIED PHYSICS LETTERS
LA English
DT Article
ID PEROVSKITE; SYSTEM; OXIDES
AB Epitaxial SrFeO3-delta (SFO) thin films have been grown on various substrates by pulsed laser deposition. The structural and electrical properties of SFO thin films are monitored with time in different atmospheres at room temperature, showing time-dependent crystal structure and electrical conductivity. The increased out-of-plane lattice parameter and resistivity over time are associated with the increased oxygen vacancies density in SFO thin films. The epitaxial strain plays an important role in determining the initial resistivity, and the sample environment determines the trend of resistivity change over time. An amorphous Al2O3 passivation layer has been found to be effective in stabilizing the structure and electrical properties of SFO thin films. This work explores time dependent structure and properties variation in oxide films and provides a way to stabilize thin film materials that are sensitive to oxygen vacancies. Published by AIP Publishing.
C1 [Enriquez, Erik; Chen, Aiping; Harrell, Zach; Lu, Xujie; Dowden, Paul; Koskelo, Nicholas; Jia, Quanxi] Los Alamos Natl Lab, Ctr Integrated Nanotechnol CINT, Los Alamos, NM 87545 USA.
[Harrell, Zach; Chen, Chonglin] Univ Texas San Antonio, Dept Phys & Astron, San Antonio, TX 78249 USA.
[Janoschek, Marc] Los Alamos Natl Lab, Condensed Matter & Magnet Sci Grp, Los Alamos, NM 87545 USA.
[Jia, Quanxi] SUNY Buffalo, Dept Mat Design & Innovat, Buffalo, NY 14260 USA.
RP Enriquez, E (reprint author), Los Alamos Natl Lab, Ctr Integrated Nanotechnol CINT, Los Alamos, NM 87545 USA.
EM emenriquez@lanl.gov; apchen@lanl.gov; qxjia@buffalo.edu
RI Lu, Xujie/L-9672-2014; Chen, Aiping/F-3212-2011
OI Lu, Xujie/0000-0001-8402-7160; Chen, Aiping/0000-0003-2639-2797
FU NNSA's Laboratory Directed Research and Development Program; U.S.
Department of Energy [DE-AC52-06NA25396]
FX The work at Los Alamos National Laboratory was supported by the NNSA's
Laboratory Directed Research and Development Program and was performed,
in part, at the Center for Integrated Nanotechnologies, an Office of
Science User Facility operated for the U.S. Department of Energy (DOE)
Office of Science. Los Alamos National Laboratory, an affirmative action
equal opportunity employer, is operated by Los Alamos National Security,
LLC, for the National Nuclear Security Administration of the U.S.
Department of Energy under Contract No. DE-AC52-06NA25396.
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PI MELVILLE
PA 1305 WALT WHITMAN RD, STE 300, MELVILLE, NY 11747-4501 USA
SN 0003-6951
EI 1077-3118
J9 APPL PHYS LETT
JI Appl. Phys. Lett.
PD OCT 3
PY 2016
VL 109
IS 14
AR 141906
DI 10.1063/1.4964384
PG 5
WC Physics, Applied
SC Physics
GA DZ8WJ
UT WOS:000386152800016
ER
PT J
AU Li, C
Zhang, YY
Pennycook, TJ
Wu, YL
Lupini, AR
Paudel, N
Pantelides, ST
Yan, YF
Pennycook, SJ
AF Li, Chen
Zhang, Yu-Yang
Pennycook, Timothy J.
Wu, Yelong
Lupini, Andrew R.
Paudel, Naba
Pantelides, Sokrates T.
Yan, Yanfa
Pennycook, Stephen J.
TI Column-by-column observation of dislocation motion in CdTe: Dynamic
scanning transmission electron microscopy
SO APPLIED PHYSICS LETTERS
LA English
DT Article
ID SCREW DISLOCATIONS; CARBON NANOTUBES; MOLECULAR-DYNAMICS;
ATOMIC-STRUCTURE; SILICON; GRAPHENE; SEMICONDUCTORS; EMISSION; BEHAVIOR;
SCALE
AB The dynamics of partial dislocations in CdTe have been observed at the atomic scale using aberration-corrected scanning transmission electron microscopy (STEM), allowing the mobility of different dislocations to be directly compared: Cd-core Shockley partial dislocations are more mobile than Te-core partials, and dislocation cores with unpaired columns have higher mobility than those without unpaired columns. The dynamic imaging also provides insight into the process by which the dislocations glide. Dislocations with dangling bonds on unpaired columns are found to be more mobile because the dangling bonds mediate the bond exchanges required for the dislocations to move. Furthermore, a screw dislocation has been resolved to dissociate into a Shockley partial-dislocation pair along two different directions, revealing a way for the screw dislocation to glide in the material. The results show that dynamic STEM imaging has the potential to uncover the details of dislocation motion not easily accessible by other means. Published by AIP Publishing.
C1 [Li, Chen] Univ Vienna, Dept Lithospher Res, A-1090 Vienna, Austria.
[Zhang, Yu-Yang; Lupini, Andrew R.; Pantelides, Sokrates T.] Oak Ridge Natl Lab, Mat Sci & Technol Div, Oak Ridge, TN 37831 USA.
[Zhang, Yu-Yang; Pantelides, Sokrates T.] Vanderbilt Univ, Dept Phys & Astron, Nashville, TN 37235 USA.
[Pennycook, Timothy J.] Univ Vienna, Fac Phys, Boltzmanngasse 5, A-1090 Vienna, Austria.
[Wu, Yelong; Paudel, Naba; Yan, Yanfa] Univ Toledo, Dept Phys & Astron, Toledo, OH 43606 USA.
[Pantelides, Sokrates T.] Vanderbilt Univ, Dept Elect Engn & Comp Sci, Nashville, TN 37235 USA.
[Pennycook, Stephen J.] Natl Univ Singapore, Dept Mat Sci & Engn, Singapore 117575, Singapore.
[Wu, Yelong] Xi An Jiao Tong Univ, Dept Appl Phys, Xian 710049, Shaanxi, Peoples R China.
RP Li, C (reprint author), Univ Vienna, Dept Lithospher Res, A-1090 Vienna, Austria.
EM lichen0320@gmail.com
RI Zhang, Yu-Yang/F-2078-2011;
OI Zhang, Yu-Yang/0000-0002-9548-0021; Li, Chen/0000-0001-9839-6100
FU U.S. DOE, Office of Energy Efficiency and Renewable Energy, Foundational
Program to Advance Cell Efficiency (F-PACE) [DE-FOA-0000492]; Office of
DOE-BES, Materials Science and Engineering Division; DOE
[DE-FG02-09ER46554]; ORNL's Center for Nanophase Materials Sciences
(CNMS) - DOE-BES; DOE Office of Science [DE-AC02-05CH11231]; National
Science Foundation [ACI-1053575]; European Union [656378, 655760]
FX This research was sponsored by the U.S. DOE, Office of Energy Efficiency
and Renewable Energy, Foundational Program to Advance Cell Efficiency
(F-PACE, DE-FOA-0000492), (CL, YLW, NP, YFY, SJP), the Office of
DOE-BES, Materials Science and Engineering Division (ARL), DOE Grant No.
DE-FG02-09ER46554 (YYZ, STP), and a user project supported by ORNL's
Center for Nanophase Materials Sciences (CNMS), which is also sponsored
by DOE-BES. Supercomputer time was provided by the National Center for
Supercomputing Applications which is supported by the DOE Office of
Science under Contract No. DE-AC02-05CH11231, and the Extreme Science
and Engineering Discovery Environment (XSEDE), which is supported by
National Science Foundation Grant No. ACI-1053575. Chen Li [No. 656378]
and Timothy Pennycook [No. 655760] are currently funded by the European
Union's Marie Sklodowska-Curie Grants.
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PI MELVILLE
PA 1305 WALT WHITMAN RD, STE 300, MELVILLE, NY 11747-4501 USA
SN 0003-6951
EI 1077-3118
J9 APPL PHYS LETT
JI Appl. Phys. Lett.
PD OCT 3
PY 2016
VL 109
IS 14
AR 143107
DI 10.1063/1.4963765
PG 5
WC Physics, Applied
SC Physics
GA DZ8WJ
UT WOS:000386152800050
ER
PT J
AU Lim, K
Schelhas, LT
Siah, SC
Brandt, RE
Zakutayev, A
Lany, S
Gorman, B
Sun, CJ
Ginley, D
Buonassisi, T
Toney, MF
AF Lim, K.
Schelhas, L. T.
Siah, S. C.
Brandt, R. E.
Zakutayev, A.
Lany, S.
Gorman, B.
Sun, C. J.
Ginley, D.
Buonassisi, T.
Toney, M. F.
TI The effect of sub-oxide phases on the transparency of tin-doped gallium
oxide
SO APPLIED PHYSICS LETTERS
LA English
DT Article
ID SOLAR-BLIND PHOTODETECTORS; BETA-GA2O3 THIN-FILMS; BUFFER LAYER; ATOMIC
LAYER; GA2O3
AB There have been a number of studies on the fabrication of Sn-doped gallium oxide (Ga2O3:Sn) films with both conductive and transparent properties using a variety of deposition methods. However, often, synthesis results in films that are not transparent. In this paper, we examine the mechanisms underlying these results in Ga2O3: Sn thin films prepared at various growth temperatures, Sn concentrations, and oxygen partial pressures. With X-ray absorption spectroscopy, transmission electron microscopy and energy dispersive spectroscopy, we find that when films are grown under the oxygen deficient conditions there are Ga sub-oxide and SnOx phases in the Ga2O3:Sn thin film. These Ga sub-oxide phases are only found in non-transparent films, and so we infer that the Ga sub-oxide is responsible for the non-transparency. These observations suggest that to obtain transparent Ga2O3:Sn, films deposition or subsequent annealing must be carefully controlled in both temperature and oxygen partial pressure to avoid the formation of Ga sub-oxide phases. Published by AIP Publishing.
C1 [Lim, K.] Stanford Univ, Dept Mat Sci & Engn, Stanford, CA 94305 USA.
[Lim, K.; Schelhas, L. T.; Toney, M. F.] SLAC Natl Accelerator Lab, Stanford Synchrotron Radiat Lightsource, Menlo Pk, CA 94025 USA.
[Siah, S. C.; Brandt, R. E.; Buonassisi, T.] MIT, 77 Massachusetts Ave, Cambridge, MA 02139 USA.
[Zakutayev, A.; Lany, S.; Ginley, D.] Natl Renewable Energy Lab, Golden, CO 80401 USA.
[Gorman, B.] Colorado Sch Mines, Dept Mat Sci & Engn, Golden, CO 80401 USA.
[Sun, C. J.] Argonne Natl Lab, Adv Photon Source, Lemont, IL 60439 USA.
RP Lim, K (reprint author), Stanford Univ, Dept Mat Sci & Engn, Stanford, CA 94305 USA.
FU Center for Next Generation Materials by Design (CNGMD), an Energy
Frontier Research Center - U.S. Department of Energy, Office of Science,
Basic Energy Science [DE-AC36-08GO28308]; U.S. Department of Energy,
Office of Basic Energy Sciences [DE-AC02-76SF00515, DE-AC02-06CH11357];
Kwanjeong Education Foundation; NRF Singapore; NSF Graduate Research
Fellowship
FX This work was supported as part of the Center for Next Generation
Materials by Design (CNGMD), an Energy Frontier Research Center funded
by the U.S. Department of Energy, Office of Science, Basic Energy
Science under Contract No. DE-AC36-08GO28308. Use of the Stanford
Synchrotron Radiation Lightsource (SLAC National Accelerator Laboratory)
was supported by the U.S. Department of Energy, Office of Basic Energy
Sciences under Contract No. DE-AC02-76SF00515. Use of the Advanced
Photon Source (Argonne National Laboratory) was supported by the U.S.
Department of Energy, Office of Basic Energy Sciences under Contract No.
DE-AC02-06CH11357. W. Tumas (NREL), M. Kolpak (MIT), and W. C. Chueh
(Stanford) are thanked for helpful discussions. K.L., S.C.S., and R.E.B.
acknowledge a Kwanjeong Education Foundation Fellowship, a Clean Energy
Scholarship from NRF Singapore, and an NSF Graduate Research Fellowship,
respectively.
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PA 1305 WALT WHITMAN RD, STE 300, MELVILLE, NY 11747-4501 USA
SN 0003-6951
EI 1077-3118
J9 APPL PHYS LETT
JI Appl. Phys. Lett.
PD OCT 3
PY 2016
VL 109
IS 14
AR 141909
DI 10.1063/1.4964638
PG 5
WC Physics, Applied
SC Physics
GA DZ8WJ
UT WOS:000386152800019
ER
PT J
AU Mahurin, SM
Mamontov, E
Thompson, MW
Zhang, PF
Turner, CH
Cummings, PT
Dai, S
AF Mahurin, Shannon M.
Mamontov, Eugene
Thompson, Matthew W.
Zhang, Pengfei
Turner, C. Heath
Cummings, Peter T.
Dai, Sheng
TI Relationship between pore size and reversible and irreversible
immobilization of ionic liquid electrolytes in porous carbon under
applied electric potential
SO APPLIED PHYSICS LETTERS
LA English
DT Article
ID GAS SEPARATION PROPERTIES; DOUBLE-LAYER; MESOPOROUS CARBON; FORCE-FIELD;
FAST DIFFUSION; CAPACITANCE; DYNAMICS; SIMULATION; CHALLENGES;
SCATTERING
AB Transport of electrolytes in nanoporous carbon-based electrodes largely defines the function and performance of energy storage devices. Using molecular dynamics simulation and quasielastic neutron scattering, we investigate the microscopic dynamics of a prototypical ionic liquid electrolyte, [emim][Tf2N], under applied electric potential in carbon materials with 6.7 nm and 1.5 nm pores. The simulations demonstrate the formation of dense layers of counter-ions near the charged surfaces, which is reversible when the polarity is reversed. In the experiment, the ions immobilized near the surface manifest themselves in the elastic scattering signal. The experimentally observed ion immobilization near the wall is fully reversible as a function of the applied electric potential in the 6.7 nm, but not in the 1.5 nm nanopores. In the latter case, remarkably, the first application of the electric potential leads to apparently irreversible immobilization of cations or anions, depending on the polarity, near the carbon pore walls. This unexpectedly demonstrates that in carbon electrode materials with the small pores, which are optimal for energy storage applications, the polarity of the electrical potential applied for the first time after the introduction of an ionic liquid electrolyte may define the decoration of the small pore walls with ions for prolonged periods of time and possibly for the lifetime of the electrode. Published by AIP Publishing.
C1 [Mahurin, Shannon M.; Zhang, Pengfei; Dai, Sheng] Oak Ridge Natl Lab, Div Chem Sci, Oak Ridge, TN 37831 USA.
[Mamontov, Eugene] Oak Ridge Natl Lab, Chem & Engn Mat Div, Oak Ridge, TN 37831 USA.
[Thompson, Matthew W.; Cummings, Peter T.] Vanderbilt Univ, Dept Chem & Biomol Engn, Nashville, TN 37235 USA.
[Turner, C. Heath] Univ Alabama, Dept Chem & Biol Engn, Tuscaloosa, AL 35487 USA.
[Dai, Sheng] Univ Tennessee, Dept Chem, Knoxville, TN 37996 USA.
RP Mahurin, SM (reprint author), Oak Ridge Natl Lab, Div Chem Sci, Oak Ridge, TN 37831 USA.
RI Mamontov, Eugene/Q-1003-2015;
OI Mamontov, Eugene/0000-0002-5684-2675; Thompson, Matthew
W./0000-0002-1460-3983
FU Fluid Interface Reactions, Structures and Transport (FIRST) Center, an
Energy Frontier Research Center - U.S. Department of Energy, Office of
Science, Office of Basic Energy Sciences; U.S. Department of Energy
[DE-AC05-00OR22725]; Department of Energy
FX This work was supported as part of the Fluid Interface Reactions,
Structures and Transport (FIRST) Center, an Energy Frontier Research
Center funded by the U.S. Department of Energy, Office of Science,
Office of Basic Energy Sciences. The neutron scattering experiments at
Oak Ridge National Laboratory's (ORNL) Spallation Neutron Source were
supported by the Scientific User Facilities Division, Office of Basic
Energy Sciences, U.S. Department of Energy. This manuscript has been
authored by UT-Battelle, LLC under Contract No. DE-AC05-00OR22725 with
the U.S. Department of Energy. The United States Government retains and
the publisher, by accepting the article for publication, acknowledges
that the United States Government retains a non-exclusive, paid-up,
irrevocable, world-wide license to publish or reproduce the published
form of this manuscript, or allow others to do so, for United States
Government purposes. The Department of Energy will provide public access
to these results of federally sponsored research in accordance with the
DOE Public Access Plan
(http://energy.gov/downloads/doe-public-access-plan).
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PI MELVILLE
PA 1305 WALT WHITMAN RD, STE 300, MELVILLE, NY 11747-4501 USA
SN 0003-6951
EI 1077-3118
J9 APPL PHYS LETT
JI Appl. Phys. Lett.
PD OCT 3
PY 2016
VL 109
IS 14
AR 143111
DI 10.1063/1.4964130
PG 5
WC Physics, Applied
SC Physics
GA DZ8WJ
UT WOS:000386152800054
ER
PT J
AU Sun, GY
Cao, X
Gao, X
Long, SW
Liang, MS
Jin, P
AF Sun, Guangyao
Cao, Xun
Gao, Xiang
Long, Shiwei
Liang, Mengshi
Jin, Ping
TI Structure and enhanced thermochromic performance of low-temperature
fabricated VO2/V2O3 thin film
SO APPLIED PHYSICS LETTERS
LA English
DT Article
ID METAL-INSULATOR-TRANSITION; OPTICAL-PROPERTIES; VANADIUM DIOXIDE;
LOW-EMISSIVITY; VO2 FILMS; PHASE; SAPPHIRE; GROWTH; LAYER; TIO2
AB For VO2-based smart window manufacture, it is a long-standing demand for high-quality thin films deposited at low temperature. Here, the thermochromic films of VO2 were deposited by a magnetron sputtering method at a fairly low temperature of 250 degrees C without subsequent annealing by embedding a V2O3 interlayer. V2O3 acts as a seed layer to lower the depositing temperature and buffer layer to epitaxial grow VO2 film. The VO2/V2O3 films display high solar modulating ability and narrow hysteresis loop. Our data can serve as a promising point for industrial production with high degree of crystallinity at a low temperature. Published by AIP Publishing.
C1 [Sun, Guangyao; Cao, Xun; Long, Shiwei; Liang, Mengshi; Jin, Ping] Chinese Acad Sci, Shanghai Inst Ceram, State Key Lab High Performance Ceram & Superfine, Dingxi 1295, Shanghai 200050, Peoples R China.
[Gao, Xiang] Oak Ridge Natl Lab, Mat Sci & Technol Div, Thin Films & Nanostruct Grp, 1 Bethel Valley Rd, Oak Ridge, TN 37831 USA.
[Jin, Ping] Natl Inst Adv Ind Sci & Technol, Mat Res Inst Sustainable Dev, Nagoya, Aichi 4638560, Japan.
RP Cao, X (reprint author), Chinese Acad Sci, Shanghai Inst Ceram, State Key Lab High Performance Ceram & Superfine, Dingxi 1295, Shanghai 200050, Peoples R China.
EM caoxun2015@gmail.com
FU Science and Technology Commission of Shanghai Municipality (STCSM)
[14DZ2261203, 5157021410]
FX This study was financially supported by the Science and Technology
Commission of Shanghai Municipality (STCSM, Nos. 14DZ2261203 and
5157021410).
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PU AMER INST PHYSICS
PI MELVILLE
PA 1305 WALT WHITMAN RD, STE 300, MELVILLE, NY 11747-4501 USA
SN 0003-6951
EI 1077-3118
J9 APPL PHYS LETT
JI Appl. Phys. Lett.
PD OCT 3
PY 2016
VL 109
IS 14
AR 143903
DI 10.1063/1.4964432
PG 5
WC Physics, Applied
SC Physics
GA DZ8WJ
UT WOS:000386152800073
ER
PT J
AU Kroll, T
Kern, J
Kubin, M
Ratner, D
Gul, S
Fuller, FD
Lochel, H
Krzywinski, J
Lutman, A
Ding, YT
Dakovski, GL
Moeller, S
Turner, JJ
Alonso-Mori, R
Nordlund, DL
Rehanek, J
Weniger, C
Firsov, A
Brzhezinskaya, M
Chatterjee, R
Lassalle-Kaiser, B
Sierra, RG
Laksmono, H
Hill, E
Borovik, A
Erko, A
Fohlisch, A
Mitzner, R
Yachandra, VK
Yano, J
Wernet, P
Bergmann, U
AF Kroll, Thomas
Kern, Jan
Kubin, Markus
Ratner, Daniel
Gul, Sheraz
Fuller, Franklin D.
Loechel, Heike
Krzywinski, Jacek
Lutman, Alberto
Ding, Yuantao
Dakovski, Georgi L.
Moeller, Stefan
Turner, Joshua J.
Alonso-Mori, Roberto
Nordlund, Dennis L.
Rehanek, Jens
Weniger, Christian
Firsov, Alexander
Brzhezinskaya, Maria
Chatterjee, Ruchira
Lassalle-Kaiser, Benedikt
Sierra, Raymond G.
Laksmono, Hartawan
Hill, Ethan
Borovik, Andrew
Erko, Alexei
Foehlisch, Alexander
Mitzner, Rolf
Yachandra, Vittal K.
Yano, Junko
Wernet, Philippe
Bergmann, Uwe
TI X-ray absorption spectroscopy using a self-seeded soft X-ray
free-electron laser
SO OPTICS EXPRESS
LA English
DT Article
ID COHERENT-LIGHT SOURCE; EMISSION-SPECTROSCOPY; DYNAMICS; PULSE;
INSTRUMENT; OXIDATION; GRATINGS; SCIENCE
AB X-ray free electron lasers (XFELs) enable unprecedented new ways to study the electronic structure and dynamics of transition metal systems. L-edge absorption spectroscopy is a powerful technique for such studies and the feasibility of this method at XFELs for solutions and solids has been demonstrated. However, the required x-ray bandwidth is an order of magnitude narrower than that of self-amplified spontaneous emission (SASE), and additional monochromatization is needed. Here we compare L-edge x-ray absorption spectroscopy (XAS) of a prototypical transition metal system based on monochromatizing the SASE radiation of the linac coherent light source (LCLS) with a new technique based on self-seeding of LCLS. We demonstrate how L-edge XAS can be performed using the self-seeding scheme without the need of an additional beam line monochromator. We show how the spectral shape and pulse energy depend on the undulator setup and how this affects the x-ray spectroscopy measurements. (C) 2016 Optical Society of America
C1 [Kroll, Thomas; Kern, Jan; Ratner, Daniel; Krzywinski, Jacek; Lutman, Alberto; Ding, Yuantao; Dakovski, Georgi L.; Moeller, Stefan; Turner, Joshua J.; Alonso-Mori, Roberto; Sierra, Raymond G.; Bergmann, Uwe] SLAC Natl Accelerator Lab, Linac Coherent Light Source, Menlo Pk, CA 94025 USA.
[Kroll, Thomas; Nordlund, Dennis L.] SLAC Natl Accelerator Lab, Stanford Synchrotron Radiat Lightsource, Menlo Pk, CA 94025 USA.
[Kern, Jan; Gul, Sheraz; Fuller, Franklin D.; Chatterjee, Ruchira; Yachandra, Vittal K.; Yano, Junko] Lawrence Berkeley Natl Lab, Mol Biophys & Integrated Bioimaging Div, Berkeley, CA 94720 USA.
[Kubin, Markus; Weniger, Christian; Foehlisch, Alexander; Mitzner, Rolf; Wernet, Philippe] Helmholtz Zentrum Berlin Mat & Energie GmbH, Inst Methods & Instrumentat Synchrotron Rad, D-12489 Berlin, Germany.
[Loechel, Heike; Rehanek, Jens; Firsov, Alexander; Brzhezinskaya, Maria; Erko, Alexei] Helmholtz Zentrum Berlin Mat & Energie, Inst Nanometer Opt & Technol, D-12489 Berlin, Germany.
[Rehanek, Jens] Paul Scherrer Inst, CH-5232 Villigen, Switzerland.
[Lassalle-Kaiser, Benedikt] Synchrotron SOLEIL, St Aubin BP 48, F-91192 Gif Sur Yvette, France.
[Sierra, Raymond G.; Laksmono, Hartawan; Bergmann, Uwe] SLAC Natl Accelerator Lab, Stanford PULSE Inst, Menlo Pk, CA 94025 USA.
[Hill, Ethan; Borovik, Andrew] Univ Calif Irvine, Dept Chem, 1102 Nat Sci 2, Irvine, CA 92697 USA.
[Foehlisch, Alexander] Univ Potsdam, Inst Phys & Astron, Karl Liebknecht Str 24-25, D-14476 Potsdam, Germany.
RP Bergmann, U (reprint author), SLAC Natl Accelerator Lab, Linac Coherent Light Source, Menlo Pk, CA 94025 USA.; Yachandra, VK; Yano, J (reprint author), Lawrence Berkeley Natl Lab, Mol Biophys & Integrated Bioimaging Div, Berkeley, CA 94720 USA.; Wernet, P (reprint author), Helmholtz Zentrum Berlin Mat & Energie GmbH, Inst Methods & Instrumentat Synchrotron Rad, D-12489 Berlin, Germany.; Bergmann, U (reprint author), SLAC Natl Accelerator Lab, Stanford PULSE Inst, Menlo Pk, CA 94025 USA.
EM vkyachandra@lbl.gov; jyano@lbl.gov; wernet@helmholtz-berlin.de;
bergmann@slac.stanford.edu
RI Kroll, Thomas/D-3636-2009;
OI Alexander, Fohlisch/0000-0003-4126-8233
FU Human Frontiers Science Project [RGP0063/2013]; National Institute of
Health (NIH) [GM116423, GM110501, GM55302, P41GM103393]; Department of
Energy (DOE), Office of Science, Office of Basic Energy Sciences (OBES)
[DE-AC02-05CH11231, DE-AC02-76SF00515]; Federal Ministry of Education
and Research (BMBF) [05K12CB4]; European Community
[PCIG10-GA-2011-297905]; Helmholtz Virtual Institute "Dynamic Pathways
in Multidimensional Landscapes"; LCLS; Stanford University through the
Stanford Institute for Materials Energy Sciences (SIMES); Lawrence
Berkeley National Laboratory (LBNL); University of Hamburg through the
BMBF [FSP 301]; Center for Free Electron Laser Science (CFEL); U.S.
Department of Energy, Office of Science, Office of Basic Energy Sciences
[DE-AC02-76SF00515]; DOE Office of Biological and Environmental
Research; National Institutes of Health, National Institute of General
Medical Sciences [P41GM103393]
FX Human Frontiers Science Project (RGP0063/2013); National Institute of
Health (NIH) (GM116423, GM110501, GM55302, P41GM103393); Department of
Energy (DOE), Office of Science, Office of Basic Energy Sciences (OBES)
(DE-AC02-05CH11231, DE-AC02-76SF00515); Federal Ministry of Education
and Research (BMBF) (05K12CB4); Marie Curie FP7-Reintegration-Grants
within the 7th European Community Framework Program
(PCIG10-GA-2011-297905); Helmholtz Virtual Institute "Dynamic Pathways
in Multidimensional Landscapes".; Portions of this research were carried
out on the SXR Instrument at the Linac Coherent Light Source (LCLS), a
division of SLAC National Accelerator Laboratory and an Office of
Science user facility operated by Stanford University for the U.S.
Department of Energy. The SXR Instrument is funded by a consortium whose
membership includes the LCLS, Stanford University through the Stanford
Institute for Materials Energy Sciences (SIMES), Lawrence Berkeley
National Laboratory (LBNL), University of Hamburg through the BMBF
priority Program No. FSP 301, and the Center for Free Electron Laser
Science (CFEL).; Use of the Linac Coherent Light Source (LCLS), SLAC
National Accelerator Laboratory, is supported by the U.S. Department of
Energy, Office of Science, Office of Basic Energy Sciences under
Contract No. DE-AC02-76SF00515. Use of the Stanford Synchrotron
Radiation Lightsource, SLAC National Accelerator Laboratory, is
supported by the U.S. Department of Energy, Office of Science, Office of
Basic Energy Sciences under Contract No. DE-AC02-76SF00515. The SSRL
Structural Molecular Biology Program (TK) is supported by the DOE Office
of Biological and Environmental Research, and by the National Institutes
of Health, National Institute of General Medical Sciences (including
P41GM103393). The contents of this publication are solely the
responsibility of the authors and do not necessarily represent the
official views of NIGMS or NIH.
NR 40
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PU OPTICAL SOC AMER
PI WASHINGTON
PA 2010 MASSACHUSETTS AVE NW, WASHINGTON, DC 20036 USA
SN 1094-4087
J9 OPT EXPRESS
JI Opt. Express
PD OCT 3
PY 2016
VL 24
IS 20
BP 22469
EP 22480
DI 10.1364/OE.24.022469
PG 12
WC Optics
SC Optics
GA EB7CL
UT WOS:000387543000016
PM 27828320
ER
PT J
AU Wang, XX
Lentine, A
DeRose, C
Starbuck, AL
Trotter, D
Pomerene, A
Mookherjea, S
AF Wang, Xiaoxi
Lentine, Anthony
DeRose, Christopher
Starbuck, Andrew L.
Trotter, Douglas
Pomerene, Andrew
Mookherjea, Shayan
TI Wide-range and fast thermally-tunable silicon photonic microring
resonators using the junction field effect
SO OPTICS EXPRESS
LA English
DT Article
ID RING RESONATORS; WAVE-GUIDES; LOW-POWER; PAIR GENERATION
AB Tunable silicon microring resonators with small, integrated micro-heaters which exhibit a junction field effect were made using a conventional silicon-on-insulator (SOI) photonic foundry fabrication process. The design of the resistive tuning section in the microrings included a "pinched" p-n junction, which limited the current at higher voltages and inhibited damage even when driven by a pre-emphasized voltage waveform. Dual-ring filters were studied for both large (>4.9 THz) and small (850 GHz) free-spectral ranges. Thermal red-shifting was demonstrated with microsecond-scale time constants, e.g., a dual-ring filter was tuned over 25 nm in 0.6 mu s 10%-90% transition time, and with efficiency of 3.2 mu W/GHz. (C) 2016 Optical Society of America
C1 [Wang, Xiaoxi; Mookherjea, Shayan] Univ Calif San Diego, Dept Elect & Comp Engn, La Jolla, CA 92093 USA.
[Lentine, Anthony; DeRose, Christopher; Starbuck, Andrew L.; Trotter, Douglas; Pomerene, Andrew] Sandia Natl Labs, Appl Photon Microsyst, Albuquerque, NM 87185 USA.
RP Mookherjea, S (reprint author), Univ Calif San Diego, Dept Elect & Comp Engn, La Jolla, CA 92093 USA.
EM smookherjea@ucsd.edu
FU National Science Foundation (NSF) [EEC-0812072, 1525090]; National
Aeronautics and Space Administration (NASA, Space Technology Research
Grants Program, Early Stage Innovations)
FX National Science Foundation (NSF) (EEC-0812072, 1525090); National
Aeronautics and Space Administration (NASA, Space Technology Research
Grants Program, Early Stage Innovations).
NR 35
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U1 7
U2 7
PU OPTICAL SOC AMER
PI WASHINGTON
PA 2010 MASSACHUSETTS AVE NW, WASHINGTON, DC 20036 USA
SN 1094-4087
J9 OPT EXPRESS
JI Opt. Express
PD OCT 3
PY 2016
VL 24
IS 20
BP 23081
EP 23093
DI 10.1364/OE.24.023081
PG 13
WC Optics
SC Optics
GA EB7CL
UT WOS:000387543000071
PM 27828374
ER
PT J
AU Mishra, V
Hirschfeld, PJ
AF Mishra, V.
Hirschfeld, P. J.
TI Effect of disorder on the competition between nematic and
superconducting order in FeSe
SO NEW JOURNAL OF PHYSICS
LA English
DT Article
DE superconductivity; nematic order; disorder effect
ID POMERANCHUK INSTABILITY; IRON PNICTIDES; CHALCOGENIDES; SYMMETRY; PHASE;
FILMS
AB Crystalline FeSe is known to display strong nematic order below a weak tetragonal-orthorhombic structural transition around T-s similar to 90 K, and a superconducting transition at T-c similar to 9 K. Recently, it was shown that electron irradiation, which creates pointlike potential scattering defects, has the surprising effect of enhancing T-c while suppressing T-s. Here we discuss a possible scenario for such an effect, which postulates a competition between s(+/-) superconductivity and nematic order. The transition to the nematic state is modeled by a mean field theory of a d-wave Pomeranchuk instability, together with a Cooper pairing interaction in both one-and multiband models. The effect of nonmagnetic impurities on both orders is treated on equal footing within the Born approximation. We find evidence that disorder can indeed enhance T-c while suppressing the competing nematic order, but only in a multiband situation. We discuss our results in the context of experimental data on FeSe crystals.
C1 [Mishra, V.] Oak Ridge Natl Lab, Comp Sci & Math Div, Oak Ridge, TN 37831 USA.
[Hirschfeld, P. J.] Univ Florida, Dept Phys, Gainesville, FL 32611 USA.
RP Mishra, V (reprint author), Oak Ridge Natl Lab, Comp Sci & Math Div, Oak Ridge, TN 37831 USA.
EM mishrav@ornl.gov; pjh@phys.ufl.edu
FU Laboratory Directed Research and Development Program of Oak Ridge
National Laboratory; [NSF-DMR-1407502]
FX The authors would like to dedicate this paper to Florence
Rullier-Albenque, whose pioneering studies of electron irradiation
disorder in correlated electron systems inspired them. The authors are
grateful for useful discussions with B M Andersen, M H Christensen, I
Paul and R Prozorov. PJH was supported by NSF-DMR-1407502. VM was
supported by the Laboratory Directed Research and Development Program of
Oak Ridge National Laboratory, managed by UT-Battelle, LLC, for the U S
Department of Energy.
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PU IOP PUBLISHING LTD
PI BRISTOL
PA TEMPLE CIRCUS, TEMPLE WAY, BRISTOL BS1 6BE, ENGLAND
SN 1367-2630
J9 NEW J PHYS
JI New J. Phys.
PD OCT 3
PY 2016
VL 18
AR 103001
DI 10.1088/1367-2630/18/10/103001
PG 11
WC Physics, Multidisciplinary
SC Physics
GA EA1LI
UT WOS:000386353300001
ER
PT J
AU Pan, Z
Chen, J
Yu, RZ
Yamamoto, H
Rong, YC
Hu, L
Li, Q
Lin, K
You, L
Zhao, K
Fan, LL
Ren, Y
Kato, K
Azuma, M
Xing, XR
AF Pan, Zhao
Chen, Jun
Yu, Runze
Yamamoto, Hajime
Rong, Yangchun
Hu, Lei
Li, Qiang
Lin, Kun
You, Li
Zhao, Kun
Fan, Longlong
Ren, Yang
Kato, Kenichi
Azuma, Masaki
Xing, Xianran
TI Giant Polarization and High Temperature Monoclinic Phase in a Lead-Free
Perovskite of Bi(Zn0.5Ti0.5)O-3-BiFeO3
SO INORGANIC CHEMISTRY
LA English
DT Article
ID SOLID-SOLUTION; ELECTRICAL-PROPERTIES; CERAMICS; FERROELECTRICS;
DEPENDENCE; TRANSITION; CRYSTAL; STATE
AB Lead-free piezoelectrics have attracted increasing attention because of the awareness of lead toxicity to the environment. Here, a new bismuth-based lead-free perovskite, (1 - x)Bi(Zn0.5Ti0.5)O-3-xBiFeO(3), has been synthesized via a high-pressure and high-temperature method. It exhibits interesting properties of giant polarization, morphotropic phase boundary (MPB), and monoclinic phase. In particular, large tetragonality (c/a = 1.228) and giant spontaneous polarization of 110 mu C/cm(2) has been obtained in 0.6 Bi(Zn0.5Ti0.5)O-3-0.4BiFeO(3), which is much higher than most available lead-free materials conventional Pb(Zr,Ti)O-3. MPB is clearly identified to be constituted of tetragonal and monoclinic phases at x = 0.5. Notably, a single monoclinic phase has been observed at x = 0.6, which exhibits an intriguing high-temperature property. The present results are helpful to explore new lead-free MPB systems in bismuth-based compounds.
C1 [Pan, Zhao; Chen, Jun; Rong, Yangchun; Hu, Lei; Li, Qiang; Lin, Kun; Zhao, Kun; Fan, Longlong; Xing, Xianran] Univ Sci & Technol Beijing, Dept Phys Chem, Beijing 100083, Peoples R China.
[You, Li] Univ Sci & Technol Beijing, State Key Lab Adv Met & Mat, Beijing 100083, Peoples R China.
[Chen, Jun; Yu, Runze; Yamamoto, Hajime; Azuma, Masaki] Tokyo Inst Technol, Mat & Struct Lab, Midori Ku, 4259 Nagatsuta, Yokohama, Kanagawa 2268503, Japan.
[Ren, Yang] Argonne Natl Lab, Xray Sci Div, 9700 S Cass Ave, Argonne, IL 60439 USA.
[Kato, Kenichi] RIKEN, SPring Ctr 8, 1-1-1 Kouto, Sayo, Hyogo 6795148, Japan.
RP Chen, J (reprint author), Univ Sci & Technol Beijing, Dept Phys Chem, Beijing 100083, Peoples R China.; Chen, J (reprint author), Tokyo Inst Technol, Mat & Struct Lab, Midori Ku, 4259 Nagatsuta, Yokohama, Kanagawa 2268503, Japan.
EM junchen@ustb.edu.cn
FU National Natural Science Foundation of China [21322102, 21590793,
91422301, 21231001]; National Program for Support of Top-notch Young
Professionals; Program for Chang Jiang Young Scholars; Fundamental
Research Funds for the Central Universities, China [FRF-TP-14-012C1];
DOE Office of Science by Argonne National Laboratory [DE-AC02-06CH11357]
FX This work was supported by the National Natural Science Foundation of
China (Grants 21322102, 21590793, 91422301, and 21231001), National
Program for Support of Top-notch Young Professionals, the Program for
Chang Jiang Young Scholars, and the Fundamental Research Funds for the
Central Universities, China (Grant FRF-TP-14-012C1). This research used
resources of the Advanced Photon Source, a U.S. Department of Energy
(DOE) Office of Science User Facility, operated for the DOE Office of
Science by Argonne National Laboratory under Contract DE-AC02-06CH11357.
The high temperature synchrotron radiation experiments were performed at
the BL44B2 of SPring-8 with the approval of the Japan Synchrotron
Radiation Research Institute (Proposals 2015B1127 and 2016A1060).
NR 30
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PU AMER CHEMICAL SOC
PI WASHINGTON
PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA
SN 0020-1669
EI 1520-510X
J9 INORG CHEM
JI Inorg. Chem.
PD OCT 3
PY 2016
VL 55
IS 19
BP 9513
EP 9516
DI 10.1021/acs.inorgchem.6b01661
PG 4
WC Chemistry, Inorganic & Nuclear
SC Chemistry
GA DY0JH
UT WOS:000384782600006
PM 27631595
ER
PT J
AU Dau, PD
Maurice, R
Renault, E
Gibson, JK
AF Dau, Phuong D.
Maurice, Remi
Renault, Eric
Gibson, John K.
TI Heptavalent Neptunium in a Gas-Phase Complex: ((NpO3+)-O-VII)(NO3-)(2)
SO INORGANIC CHEMISTRY
LA English
DT Article
ID PLUTONIUM TETROXIDE; ALKALINE-SOLUTION; BASIS-SETS; NITRATE COMPLEXES;
OXIDATION; EXCHANGE; URANYL; ION; DECOMPOSITION; DISSOCIATION
AB A central goal of chemistry is to achieve ultimate oxidation states, including in gas-phase complexes with no condensed phase perturbations. In the case of the actinide elements, the highest established oxidation states are labile Pu(VII) and somewhat more stable Np(VII). We have synthesized and characterized gas-phase AnO(3)(NO3)(2)(-) complexes for An U, Np, and Pu by endothermic NO2 elimination from AnO(2)(NO3)(3)(-). It was previously demonstrated that the PuO3+ core of PuO3(NO3)(2)(-) has a Pu-O-center dot radical bond such that the oxidation state is Pu(VI); it follows that in UO3(NO3)(2)(-) it is the stable U(VI) oxidation state. On the basis of the relatively more facile synthesis of NpO3(NO3)(2)(-)(,) a Np(VII) oxidation state is inferred. This interpretation is substantiated by reactivity of the three complexes: NO2 spontaneously adds to UO3(NO3)(2)(-) and PuO3(NO3)(2)(-) but not to NpO3(NO3)(2)(-). This unreactive character is attributed to a Np(VII)O-3(+) core with three stable Np=O bonds, this in contrast to reactive U-O-center dot and Pu-O-center dot radical bonds. The computed structures and reaction energies for the three AnO(3)(NO3)(2)(-) support the conclusion that the oxidation states are U(VI), Np(VII), and Pu(VI): The results establish the extreme Np(VII) oxidation state in a gas-phase complex, and demonstrate the inherently greater stability of Np(VII) versus Pu(VII).
C1 [Dau, Phuong D.; Gibson, John K.] Lawrence Berkeley Natl Lab, Div Chem Sci, Berkeley, CA 94720 USA.
[Maurice, Remi] Univ Nantes, EMN Nantes, IN2P3, SUBATECH,UMR CNRS 6457, 4 Rue Alfred Kastler, F-44307 Nantes 3, France.
[Renault, Eric] Univ Nantes, UMR CNRS 6230, CEISAM, 2 Rue Houssiniere,BP 92208, F-44322 Nantes 3, France.
RP Gibson, JK (reprint author), Lawrence Berkeley Natl Lab, Div Chem Sci, Berkeley, CA 94720 USA.; Maurice, R (reprint author), Univ Nantes, EMN Nantes, IN2P3, SUBATECH,UMR CNRS 6457, 4 Rue Alfred Kastler, F-44307 Nantes 3, France.
EM remi.maurice@subatech.in2p3.fr; jkgibson@lbl.gov
RI Renault, Eric/A-2474-2009
OI Renault, Eric/0000-0001-5525-812X
FU U.S. Department of Energy, Office of Basic Energy Sciences, Heavy
Element Chemistry, at LBNL [DE-AC02-05CH11231]; GENCI-CINES/IDRIS
[2015-c2015085117]
FX The work of P.D.D. and J.K.G. was fully supported by the U.S. Department
of Energy, Office of Basic Energy Sciences, Heavy Element Chemistry, at
LBNL under Contract No. DE-AC02-05CH11231. Calculations were carried out
using HPC resources from GENCI-CINES/IDRIS (grant 2015-c2015085117) and
CCIPL ("Centre de Calcul Intensif des Pays de la Loire").
NR 42
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PU AMER CHEMICAL SOC
PI WASHINGTON
PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA
SN 0020-1669
EI 1520-510X
J9 INORG CHEM
JI Inorg. Chem.
PD OCT 3
PY 2016
VL 55
IS 19
BP 9830
EP 9837
DI 10.1021/acs.inorgchem.6b01617
PG 8
WC Chemistry, Inorganic & Nuclear
SC Chemistry
GA DY0JH
UT WOS:000384782600041
PM 27631457
ER
PT J
AU Danaie, M
Kepaptsoglou, D
Ramasse, QM
Ophus, C
Whittle, KR
Lawson, SM
Pedrazzini, S
Young, NP
Bagot, PAJ
Edmondson, PD
AF Danaie, Mohsen
Kepaptsoglou, Demie
Ramasse, Quentin M.
Ophus, Colin
Whittle, Karl R.
Lawson, Sebastian M.
Pedrazzini, Stella
Young, Neil P.
Bagot, Paul A. J.
Edmondson, Philip D.
TI Characterization of Ordering in A-Site Deficient Perovskite
Ca1-xLa2x/3TiO3 Using STEM/EELS
SO INORGANIC CHEMISTRY
LA English
DT Article
ID CRYSTAL-STRUCTURE; ELECTRON-DIFFRACTION; PHASE-TRANSITION; X-RAY;
SYSTEM; LANTHANUM; CATIO3; OXIDES; TILT; MICROSTRUCTURE
AB The vacancy ordering behavior of an A-site deficient perovskite system, Ca1-xLa2x/3TiO3, was studied using atomic resolution scanning transmission electron microscopy (STEM) in conjunction with electron energy-loss spectroscopy (EELS), with the aim of determining the role of A-site composition changes. At low La content (x = 0.2), adopting Pbnm symmetry, there was no indication of long-range ordering. Domains, with clear boundaries, were observed in bright-field (BF) imaging, but were not immediately visible in the corresponding high-angle annular dark-field (HAADF) image. These boundaries, with the aid of displacement maps from A-site cations in the HAADF signal, are shown to be tilt boundaries. At the La-rich end of the composition (x = 0.9), adopting Cmmm symmetry, long-range ordering of vacancies and La3+ ions was observed, with alternating La-rich and La-poor layers on (001)(p) planes, creating a double perovskite lattice along the c axis. These highly ordered domains can be found isolated within a random distribution of vacancies/La3+, or within a large population, encompassing a large volume. In regions with a high number density of double perovskite domains, these highly ordered domains were separated by twin boundaries, with 90 degrees or 180 degrees lattice rotations across boundaries. The occurrence and characteristics of these ordered structures are discussed and compared with similar perovskite systems.
C1 [Danaie, Mohsen; Pedrazzini, Stella; Young, Neil P.; Bagot, Paul A. J.] Univ Oxford, Dept Mat, Parks Rd, Oxford OX1 3PH, England.
[Kepaptsoglou, Demie; Ramasse, Quentin M.] SuperSTEM Lab, SciTech Daresbury Campus, Warrington WA4 4AD, Cheshire, England.
[Ophus, Colin] Lawrence Berkeley Natl Lab, Natl Ctr Electron Microscopy, Mol Foundry, 67 Cyclotron Rd, Berkeley, CA 94720 USA.
[Whittle, Karl R.; Lawson, Sebastian M.] Univ Sheffield, Dept Mat Sci & Engn, Immobilisat Sci Lab, Mappin St, Sheffield S1 3JD, S Yorkshire, England.
[Whittle, Karl R.] Univ Liverpool, Sch Engn, Brownlow Hill, Liverpool L69 3GH, Merseyside, England.
[Edmondson, Philip D.] Oak Ridge Natl Lab, Div Mat Sci & Technol, 1 Bethel Valley Rd, Oak Ridge, TN 37831 USA.
RP Danaie, M (reprint author), Univ Oxford, Dept Mat, Parks Rd, Oxford OX1 3PH, England.
EM mohsen.danaie@materials.ox.ac.uk
FU UK's Engineering and Physical Sciences Research Council (EPSRC)
[EP/K029770/1, EP/L005581/1]; U.S. Department of Energy, Office of
Science, Fusion Energy Sciences; EPSRC [EP/G037140/1]; Office of
Science, Office of Basic Energy Sciences, of the U.S. Department of
Energy [DE-AC02-05CH11231]
FX Funding is acknowledged from the UK's Engineering and Physical Sciences
Research Council (EPSRC) under grants EP/K029770/1 and EP/L005581/1. PDE
acknowledges support from the U.S. Department of Energy, Office of
Science, Fusion Energy Sciences. SML acknowledges funding from the EPSRC
grant EP/G037140/1. SuperSTEM is the UK National Facility for
Aberration-Corrected STEM, supported by EPSRC. Work at the Molecular
Foundry was supported by the Office of Science, Office of Basic Energy
Sciences, of the U.S. Department of Energy under Contract No.
DE-AC02-05CH11231. Guidance in sample preparation from Amy Gandy is
gratefully acknowledged.
NR 60
TC 1
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U1 14
U2 14
PU AMER CHEMICAL SOC
PI WASHINGTON
PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA
SN 0020-1669
EI 1520-510X
J9 INORG CHEM
JI Inorg. Chem.
PD OCT 3
PY 2016
VL 55
IS 19
BP 9937
EP 9948
DI 10.1021/acs.inorgchem.6b02087
PG 12
WC Chemistry, Inorganic & Nuclear
SC Chemistry
GA DY0JH
UT WOS:000384782600051
PM 27631169
ER
PT J
AU Ge, SF
He, HJ
Xiao, RQ
AF Ge, Shao-Feng
He, Hong-Jian
Xiao, Rui-Qing
TI Probing new physics scales from Higgs and electroweak observables at
e(+) e(-) Higgs factory
SO JOURNAL OF HIGH ENERGY PHYSICS
LA English
DT Article
DE Beyond Standard Model; Higgs Physics
ID STANDARD MODEL; PHENOMENOLOGICAL LAGRANGIANS; MASSLESS PARTICLES; BROKEN
SYMMETRIES; GAUGE-THEORIES; DARK-MATTER; COUPLINGS; BOSON; CONSERVATION;
INFLATION
AB New physics beyond the standard model (SM) can be model-independently formulated via dimension-6 effective operators, whose coefficients (cutoffs) characterize the scales of new physics. We study the probe of new physics scales from the electroweak precision observables (EWPO) and the Higgs observables (HO) at the future e(+)e(-) Higgs factory (such as CEPC). To optimize constraints of new physics from all available observables, we establish a scheme-independent approach. With this formulation, we treat the SM electroweak parameters and the coefficients of dimension-6 operators on equal footing, which can be fitted simultaneously by the same chi(2) function. As deviations from the SM are generally small, we can expand the new physics parameters up to linear order and perform an analytical chi(2) fit to derive the potential reach of the new physics scales. We find that the HO from both Higgs produnction and decay rates can probe the new physics scales up to 10 TeV (and to 44 TeV for the case of gluon-involved operator O-g), and the new physics scales of Yukawa-type operators can be probed by the precision Higgs coupling measurements up to (13 - 25) TeV. Further including the EWPO can push the limit up to 35 TeV. From this prospect, we demonstrate that the EWPO measured in the early phase of a Higgs factory can be as important as the Higgs observables. These indirect probes of new physics scales at the Higgs factory can mainly cover the energy range to be directly explored by the next generation hadron colliders of pp (50 - 100TeV), such as the SPPC and FCC-hh.
C1 [Ge, Shao-Feng] Max Planck Inst Kernphys, D-69117 Heidelberg, Germany.
[He, Hong-Jian; Xiao, Rui-Qing] Tsinghua Univ, Inst Modern Phys, Beijing 100084, Peoples R China.
[He, Hong-Jian; Xiao, Rui-Qing] Tsinghua Univ, Ctr High Energy Phys, Beijing 100084, Peoples R China.
[He, Hong-Jian] Peking Univ, Ctr High Energy Phys, Beijing 100871, Peoples R China.
[Xiao, Rui-Qing] Lawrence Berkeley Natl Lab, Berkeley, CA 94720 USA.
RP Ge, SF (reprint author), Max Planck Inst Kernphys, D-69117 Heidelberg, Germany.
EM gesf02@gmail.com; hjhe@tsinghua.edu.cn; ruiqingxiao@lbl.gov
FU National NSF of China [11275101, 11135003]; Tsinghua University
[20141081211]
FX We thank Matthew McCullough, Manqi Ruan, and Tevong You for many
valuable discussions. We are grateful to Michael Peskin for discussing
the chi2 analysis of ref. [11]. We also thank Timothy
Barklow, Tao Han, Zhijun Liang, Matthew Strassler, Liantao Wang, Xinchou
Lou and Yifang Wang for discussions. SFG thanks Matthew McCullough for
kind invitation and hospitality during his visit at CERN Theory
Division. This work is supported in part by National NSF of China (under
grants 11275101 and 11135003) and by Tsinghua University (under grant
20141081211).
NR 110
TC 1
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U1 5
U2 5
PU SPRINGER
PI NEW YORK
PA 233 SPRING ST, NEW YORK, NY 10013 USA
SN 1029-8479
J9 J HIGH ENERGY PHYS
JI J. High Energy Phys.
PD OCT 3
PY 2016
IS 10
AR 007
DI 10.1007/JHEP10(2016)007
PG 48
WC Physics, Particles & Fields
SC Physics
GA DY8RH
UT WOS:000385397500002
ER
PT J
AU de Jong, M
Chen, W
Notestine, R
Persson, K
Ceder, G
Jain, A
Asta, M
Gamst, A
AF de Jong, Maarten
Chen, Wei
Notestine, Randy
Persson, Kristin
Ceder, Gerbrand
Jain, Anubhav
Asta, Mark
Gamst, Anthony
TI A Statistical Learning Framework for Materials Science: Application to
Elastic Moduli of k-nary Inorganic Polycrystalline Compounds
SO SCIENTIFIC REPORTS
LA English
DT Article
ID DENSITY-FUNCTIONAL THEORY; CRYSTAL-STRUCTURE; HIGH-THROUGHPUT; BULK
MODULI; THERMAL-CONDUCTIVITY; VOLUME RELATIONSHIP; MATERIALS DESIGN;
SOLIDS; APPROXIMATION; PREDICTIONS
AB Materials scientists increasingly employ machine or statistical learning (SL) techniques to accelerate materials discovery and design. Such pursuits benefit from pooling training data across, and thus being able to generalize predictions over, k-nary compounds of diverse chemistries and structures. This work presents a SL framework that addresses challenges in materials science applications, where datasets are diverse but of modest size, and extreme values are often of interest. Our advances include the application of power or Holder means to construct descriptors that generalize over chemistry and crystal structure, and the incorporation of multivariate local regression within a gradient boosting framework. The approach is demonstrated by developing SL models to predict bulk and shear moduli (K and G, respectively) for polycrystalline inorganic compounds, using 1,940 compounds from a growing database of calculated elastic moduli for metals, semiconductors and insulators. The usefulness of the models is illustrated by screening for superhard materials.
C1 [de Jong, Maarten; Persson, Kristin; Ceder, Gerbrand; Asta, Mark] Univ Calif Berkeley, Dept Mat Sci & Engn, Berkeley, CA 94720 USA.
[Chen, Wei; Persson, Kristin; Jain, Anubhav] Lawrence Berkeley Natl Lab, Energy Technol Area, Berkeley, CA 94720 USA.
[Notestine, Randy; Gamst, Anthony] Univ Calif San Diego, San Diego Supercomp Ctr, Computat & Appl Stat Lab, La Jolla, CA 92093 USA.
[Ceder, Gerbrand; Asta, Mark] Lawrence Berkeley Natl Lab, Mat Sci Div, Berkeley, CA 94720 USA.
[de Jong, Maarten] Space Explorat Technol, 1 Rocket Rd, Hawthorne, CA 90250 USA.
[Chen, Wei] IIT, Dept Mech Mat & Aerosp Engn, Chicago, IL 60616 USA.
RP de Jong, M (reprint author), Univ Calif Berkeley, Dept Mat Sci & Engn, Berkeley, CA 94720 USA.; de Jong, M (reprint author), Space Explorat Technol, 1 Rocket Rd, Hawthorne, CA 90250 USA.
EM maartendft@gmail.com
RI Chen, Wei/B-3045-2012
OI Chen, Wei/0000-0002-1135-7721
FU Department of Energy Basic Energy Sciences program - the Materials
Project [EDCBEE]; Office of Science of the U.S. Department of Energy
[DEAC02-05CH11231]
FX This work was intellectually led by the Department of Energy Basic
Energy Sciences program - the Materials Project - under Grant No.
EDCBEE. Work at Lawrence Berkeley was supported by the Office of Science
of the U.S. Department of Energy under Contract No. DEAC02-05CH11231.
The authors thank Shyue Ping Ong for assistance with pymatgen and his
extensive contributions to both pymatgen and the Materials Project.
NR 68
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U1 24
U2 24
PU NATURE PUBLISHING GROUP
PI LONDON
PA MACMILLAN BUILDING, 4 CRINAN ST, LONDON N1 9XW, ENGLAND
SN 2045-2322
J9 SCI REP-UK
JI Sci Rep
PD OCT 3
PY 2016
VL 6
AR 34256
DI 10.1038/srep34256
PG 11
WC Multidisciplinary Sciences
SC Science & Technology - Other Topics
GA DX9ZY
UT WOS:000384757600001
PM 27694824
ER
PT J
AU Brahlek, M
Koirala, N
Salehi, M
Moon, J
Zhang, WH
Li, HX
Zhou, XQ
Han, MG
Wu, L
Emge, T
Lee, HD
Xu, C
Rhee, SJ
Gustafsson, T
Armitage, NP
Zhu, YM
Dessau, DS
Wu, WD
Oh, S
AF Brahlek, Matthew
Koirala, Nikesh
Salehi, Maryam
Moon, Jisoo
Zhang, Wenhan
Li, Haoxiang
Zhou, Xiaoqing
Han, Myung-Geun
Wu, Liang
Emge, Thomas
Lee, Hang-Dong
Xu, Can
Rhee, Seuk Joo
Gustafsson, Torgny
Armitage, N. Peter
Zhu, Yimei
Dessau, Daniel S.
Wu, Weida
Oh, Seongshik
TI Disorder-driven topological phase transition in Bi2Se3 films
SO PHYSICAL REVIEW B
LA English
DT Article
ID SPIN TEXTURE; INSULATOR; DIFFUSION; ABSENCE
AB Topological insulators (TI) are a phase of matter that host unusual metallic surface states. Unlike the states that exist on the surface of conventional materials, these so-called topological surfaces states (TSS) are protected against disorder-related localization effects by time reversal symmetry through strong spin-orbit coupling. By combining transport measurements, angle-resolved photoemission spectroscopy, and scanning tunneling microscopy, we show that there exists a critical level of disorder beyond which the TI Bi2Se3 loses its ability to protect the metallic TSS and transitions to a fully insulating state. The absence of the metallic surface channels dictates that there is a change in the material's topological character, implying that disorder can lead to a topological phase transition even without breaking the time reversal symmetry. This observation challenges the conventional notion of topologically protected surface states and should prompt new studies as to the fundamental nature of topological phase of matter in the presence of disorder.
C1 [Brahlek, Matthew; Koirala, Nikesh; Moon, Jisoo; Zhang, Wenhan; Lee, Hang-Dong; Xu, Can; Gustafsson, Torgny; Wu, Weida; Oh, Seongshik] Rutgers State Univ, Dept Phys & Astron, Piscataway, NJ 08854 USA.
[Salehi, Maryam] Rutgers State Univ, Dept Mat Sci & Engn, Piscataway, NJ 08854 USA.
[Li, Haoxiang; Zhou, Xiaoqing; Dessau, Daniel S.] Univ Colorado, Dept Phys, Boulder, CO 80309 USA.
[Han, Myung-Geun; Zhu, Yimei] Brookhaven Natl Lab, Condensed Matter Phys & Mat Sci, Upton, NY 11973 USA.
[Wu, Liang; Armitage, N. Peter] Johns Hopkins Univ, Dept Phys & Astron, Inst Quantum Matter, Baltimore, MD 21218 USA.
[Emge, Thomas] Rutgers State Univ, Dept Chem, POB 939, Piscataway, NJ 08854 USA.
[Rhee, Seuk Joo] Hankuk Univ Foreign Studies, Dept Phys, Yongin 449791, Kyongki Do, South Korea.
RP Oh, S (reprint author), Rutgers State Univ, Dept Phys & Astron, Piscataway, NJ 08854 USA.
EM ohsean@physics.rutgers.edu
RI Wu, Liang/C-8715-2015
OI Wu, Liang/0000-0003-1696-7809
FU National Science Foundation [DMREF-1233349, DMR-1126468, DMR-1308142,
DMR-1506618, DMR-1106070, EFMA-1542798]; Gordon and Betty Moore
Foundation's EPiQS Initiative [GBMF4418]; US Department of Energy (DOE)
[DE-FG0203ER46066]; Gordon and Betty Moore Foundation [GBMF2628]; Army
Research Office [W911NF-15-1-0560]; US DOE, Office of Basic Energy
Science, Division of Materials Science and Engineering [DESC0012704];
Office of Science, Office of Basic Energy Sciences, of the US DOE
[DE-AC02-05CH11231]
FX We thank Emil Prodan for helpful discussions. This work is supported by
the National Science Foundation (Grants No. DMREF-1233349, No.
DMR-1126468, No. DMR-1308142, No. DMR-1506618, No. DMR-1106070, and No.
EFMA-1542798), Gordon and Betty Moore Foundation's EPiQS Initiative
(GBMF4418) for S.O., US Department of Energy (DOE) (Contract No.
DE-FG0203ER46066) for D.S.D., and Gordon and Betty Moore Foundation
(GBMF2628) and Army Research Office (Grant No. W911NF-15-1-0560) for
N.P.A. The work at Brookhaven National Lab is supported by the US DOE,
Office of Basic Energy Science, Division of Materials Science and
Engineering under Contract No. DESC0012704. The transmission electron
microscopy sample preparation was carried out at the Center for
Functional Nanomaterials, Brookhaven National Laboratory. The Advanced
Light Source is supported by the Director, Office of Science, Office of
Basic Energy Sciences, of the US DOE under Contract No.
DE-AC02-05CH11231.
NR 33
TC 0
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U1 26
U2 26
PU AMER PHYSICAL SOC
PI COLLEGE PK
PA ONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA
SN 2469-9950
EI 2469-9969
J9 PHYS REV B
JI Phys. Rev. B
PD OCT 3
PY 2016
VL 94
IS 16
AR 165104
DI 10.1103/PhysRevB.94.165104
PG 5
WC Physics, Condensed Matter
SC Physics
GA DX6DA
UT WOS:000384472100006
ER
PT J
AU Kolesnikov, AI
Podlesnyak, A
Sadykov, RA
Antonov, VE
Kuzovnikov, MA
Ehlers, G
Granroth, GE
AF Kolesnikov, A. I.
Podlesnyak, A.
Sadykov, R. A.
Antonov, V. E.
Kuzovnikov, M. A.
Ehlers, G.
Granroth, G. E.
TI Pressure effect on hydrogen tunneling and vibrational spectrum in
alpha-Mn
SO PHYSICAL REVIEW B
LA English
DT Article
ID TEMPERATURE-DEPENDENCE; NEUTRON-SCATTERING; MANGANESE; STATES
AB The pressure effect on the tunneling mode and vibrational spectra of hydrogen in alpha-MnH0.07 has been studied by inelastic neutron scattering. Applying hydrostatic pressure of up to 30 kbar is shown to shift both the hydrogen optical modes and the tunneling peak to higher energies. First-principles calculations show that the potential for hydrogen in alpha-Mn becomes overall steeper with increasing pressure. At the same time, the barrier height and its extent in the direction of tunneling decrease and the calculations predict significant changes of the dynamics of hydrogen in alpha-Mn at 100 kbar, when the estimated tunneling splitting of the hydrogen ground state exceeds the barrier height.
C1 [Kolesnikov, A. I.] Oak Ridge Natl Lab, Chem & Engn Mat Div, Oak Ridge, TN 37831 USA.
[Podlesnyak, A.; Ehlers, G.] Oak Ridge Natl Lab, Quantum Condensed Matter Div, Oak Ridge, TN 37831 USA.
[Sadykov, R. A.] RAS, Inst High Pressure Phys, Troitsk 108840, Russia.
[Sadykov, R. A.] RAS, Inst Nucl Res, Moscow 117312, Russia.
[Antonov, V. E.; Kuzovnikov, M. A.] RAS, Inst Solid State Phys, Chernogolovka 142432, Moscow Region, Russia.
[Kuzovnikov, M. A.] PAS, Inst Phys Chem, PL-01224 Warsaw, Poland.
[Granroth, G. E.] Oak Ridge Natl Lab, Neutron Data Anal & Visualizat Div, Oak Ridge, TN 37831 USA.
RP Kolesnikov, AI (reprint author), Oak Ridge Natl Lab, Chem & Engn Mat Div, Oak Ridge, TN 37831 USA.
EM kolesnikovai@ornl.gov
RI Granroth, Garrett/G-3576-2012; Ehlers, Georg/B-5412-2008; Podlesnyak,
Andrey/A-5593-2013
OI Granroth, Garrett/0000-0002-7583-8778; Ehlers,
Georg/0000-0003-3513-508X; Podlesnyak, Andrey/0000-0001-9366-6319
FU Scientific User Facilities Division, Office of Basic Energy Sciences,
U.S. Department of Energy; Office of Science of the U.S. Department of
Energy [DE-AC02-05CH11231]; Laboratory Directed Research and Development
Program of Oak Ridge National Laboratory; UT-Battelle, LLC
[DE-AC05-00OR22725]; U.S. Department of Energy; DOE Public Access Plan;
Program on Elementary Particle Physics, Fundamental Nuclear Physics, and
Nuclear Technologies of RAS
FX Research at Oak Ridge National Laboratory's Spallation Neutron Source
was supported by the Scientific User Facilities Division, Office of
Basic Energy Sciences, U.S. Department of Energy. This research used
resources of the National Energy Research Scientific Computing Center,
which is supported by the Office of Science of the U.S. Department of
Energy under Contract No. DE-AC02-05CH11231. A portion of this research
was sponsored by the Laboratory Directed Research and Development
Program of Oak Ridge National Laboratory, managed by UT-Battelle, LLC,
for the U.S. Department of Energy. Support by a grant of the Program on
Elementary Particle Physics, Fundamental Nuclear Physics, and Nuclear
Technologies of RAS is also acknowledged.; This manuscript has been
authored by UT-Battelle, LLC, under Contract No. DE-AC05-00OR22725 with
the U.S. Department of Energy. The United States Government retains and
the publisher, by accepting the article for publication,acknowledges
that the United States Government retains a non-exclusive, paid-up,
irrevocable, world-wide license to publish or reproduce the published
form of this manuscript, or allow others to do so, for United States
Government purposes. The Department of Energy will provide public access
to these results of federally sponsored research in accordance with the
DOE Public Access Plan
(http://energy.gov/downloads/doe-public-access-plan).
NR 27
TC 0
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U1 13
U2 13
PU AMER PHYSICAL SOC
PI COLLEGE PK
PA ONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA
SN 2469-9950
EI 2469-9969
J9 PHYS REV B
JI Phys. Rev. B
PD OCT 3
PY 2016
VL 94
IS 13
AR 134301
DI 10.1103/PhysRevB.94.134301
PG 5
WC Physics, Condensed Matter
SC Physics
GA DX6CH
UT WOS:000384469800002
ER
PT J
AU Sjostrom, T
Crockett, S
Rudin, S
AF Sjostrom, Travis
Crockett, Scott
Rudin, Sven
TI Multiphase aluminum equations of state via density functional theory
SO PHYSICAL REVIEW B
LA English
DT Article
ID AUGMENTED-WAVE METHOD; OF-STATE; TERAPASCAL PRESSURES; LIQUID ALUMINUM;
COPPER; COMPRESSIBILITY; TANTALUM; IRON; GPA; LEAD
AB We have performed density functional theory (DFT) based calculations for aluminum in extreme conditions of both pressure and temperature, up to five times compressed ambient density, and over 1 000 000 K in temperature. In order to cover such a domain, DFT methods including phonon calculations, quantum molecular dynamics, and orbital-free DFT are employed. The results are then used to construct a SESAME equation of state for the aluminum 1100 alloy, encompassing the fcc, hcp, and bcc solid phases as well as the liquid regime. We provide extensive comparison with experiment, and based on this we also provide a slightly modified equation of state for the aluminum 6061 alloy.
C1 [Sjostrom, Travis; Crockett, Scott; Rudin, Sven] Los Alamos Natl Lab, Div Theoret, Los Alamos, NM 87545 USA.
RP Sjostrom, T (reprint author), Los Alamos Natl Lab, Div Theoret, Los Alamos, NM 87545 USA.
FU Los Alamos National Laboratory; National Nuclear Security Administration
of the U.S. Department of Energy [DE-AC52-06NA25396]
FX We would like to thank D.C. Wallace for helpful and encouraging
discussions and J.C. Lashley for providing his aluminum crystal data.
This work was performed under the auspices of Los Alamos National
Laboratory, which is operated by Los Alamos National Security, LLC, for
the National Nuclear Security Administration of the U.S. Department of
Energy under Contract No. DE-AC52-06NA25396.
NR 90
TC 0
Z9 0
U1 15
U2 15
PU AMER PHYSICAL SOC
PI COLLEGE PK
PA ONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA
SN 2469-9950
EI 2469-9969
J9 PHYS REV B
JI Phys. Rev. B
PD OCT 3
PY 2016
VL 94
IS 14
AR 144101
DI 10.1103/PhysRevB.94.144101
PG 10
WC Physics, Condensed Matter
SC Physics
GA DX6CM
UT WOS:000384470500001
ER
PT J
AU Chen, QB
Zhang, SQ
Zhao, PW
Jolos, RV
Meng, J
AF Chen, Q. B.
Zhang, S. Q.
Zhao, P. W.
Jolos, R. V.
Meng, J.
TI Two-dimensional collective Hamiltonian for chiral and wobbling modes
SO PHYSICAL REVIEW C
LA English
DT Article
ID COORDINATE METHOD; ODD NUCLEI; MOTION; BANDS; ROTATION; EXCITATIONS
AB A two-dimensional collective Hamiltonian (2DCH) on both azimuth and polar motions in triaxial nuclei is proposed to investigate the chiral and wobbling modes. In the 2DCH, the collective potential and the mass parameters are determined from three-dimensional tilted axis cranking (TAC) calculations. The broken chiral and signature symmetries in the TAC solutions are restored by the 2DCH. The validity of the 2DCH is illustrated with a triaxial rotor (gamma = -30 degrees) coupling to one h(11/2) proton particle and one h(11/2) neutron hole. By diagonalizing the 2DCH, the angular momenta and energy spectra are obtained. These results agree with the exact solutions of the particle rotor model (PRM) at high rotational frequencies. However, at low frequencies, the energies given by the 2DCH are larger than those by the PRM due to the underestimation of the mass parameters. In addition, with increasing angular momentum, the transitions from the chiral vibration to chiral rotation and further to longitudinal wobbling motion have been presented in the 2DCH.
C1 [Chen, Q. B.; Zhang, S. Q.; Meng, J.] Peking Univ, Sch Phys, State Key Lab Nucl Phys & Technol, Beijing 100871, Peoples R China.
[Zhao, P. W.] Argonne Natl Lab, Div Phys, Argonne, IL 60439 USA.
[Jolos, R. V.] Joint Inst Nucl Res, Dubna 141980, Russia.
[Jolos, R. V.] Dubna State Univ, Dubna 141980, Russia.
[Meng, J.] Beihang Univ, Sch Phys & Nucl Energy Engn, Beijing 100191, Peoples R China.
[Meng, J.] Univ Stellenbosch, Dept Phys, Stellenbosch, South Africa.
RP Zhang, SQ (reprint author), Peking Univ, Sch Phys, State Key Lab Nucl Phys & Technol, Beijing 100871, Peoples R China.
EM sqzhang@pku.edu.cn; mengj@pku.edu.cn
RI Zhao, Pengwei/F-9107-2010; Meng, Jie/B-8548-2009; Chen, Qibo/C-2054-2013
OI Zhao, Pengwei/0000-0001-8243-2381; Meng, Jie/0000-0002-0977-5318; Chen,
Qibo/0000-0001-5159-4468
FU Major State 973 Program of China [2013CB834400]; National Natural
Science Foundation of China [11335002, 11375015, 11461141002,
11621131001]; China Postdoctoral Science Foundation [2015M580007,
2016T90007]; U.S. Department of Energy (DOE), Office of Science, Office
of Nuclear Physics [DE-AC02-06CH11357]
FX We thank K. Matsuyanagi and S. Frauendorf for helpful discussions. This
work was supported in part by the Major State 973 Program of China
(Grant No. 2013CB834400), the National Natural Science Foundation of
China (Grants No. 11335002, No. 11375015, No. 11461141002, and No.
11621131001), the China Postdoctoral Science Foundation under Grants No.
2015M580007 and No. 2016T90007, and the U.S. Department of Energy (DOE),
Office of Science, Office of Nuclear Physics, under Contract No.
DE-AC02-06CH11357 (P.W.Z.). This work used the computing resources of
the Laboratory Computing Resource Center at Argonne National Laboratory.
NR 63
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U1 2
U2 2
PU AMER PHYSICAL SOC
PI COLLEGE PK
PA ONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA
SN 2469-9985
EI 2469-9993
J9 PHYS REV C
JI Phys. Rev. C
PD OCT 3
PY 2016
VL 94
IS 4
AR 044301
DI 10.1103/PhysRevC.94.044301
PG 13
WC Physics, Nuclear
SC Physics
GA DX6DE
UT WOS:000384472500001
ER
PT J
AU Aab, A
Abreu, P
Aglietta, M
Al Samarai, I
Albuquerque, IFM
Allekotte, I
Almela, A
Castillo, JA
Alvarez-Muniz, J
Ambrosio, M
Anastasi, GA
Anchordoqui, L
Andrada, B
Andringa, S
Aramo, C
Arqueros, F
Arsene, N
Asorey, H
Assis, P
Aublin, J
Avila, G
Badescu, AM
Balaceanu, A
Luz, RJB
Baus, C
Beatty, JJ
Becker, KH
Bellido, JA
Berat, C
Bertaina, E
Bertou, X
Biermann, PL
Billoir, P
Biteau, J
Blaess, SG
Blanco, A
Blazek, J
Bleve, C
Bohacova, M
Boncioli, D
Bonifazi, C
Borodai, N
Botti, AM
Brack, J
Brancus, I
Bretz, T
Bridgeman, A
Briechle, FL
Buchholz, P
Bueno, A
Buitink, S
Buscemi, M
Caballero-Mora, KS
Caccianiga, L
Cancio, A
Canfora, F
Caramete, L
Caruso, R
Castellina, A
Cataldi, G
Cazon, L
Cester, R
Chavez, AG
Chinellato, JA
Chudoba, J
Clay, RW
Colalillo, R
Coleman, A
Collica, L
Coluccia, MR
Conceicao, R
Contreras, F
Cooper, MJ
Coutu, S
Covault, CE
Cronin, J
D'Amico, S
Daniel, B
Dasso, S
Daumiller, K
Dawson, BR
de Almeida, RM
de Jong, SJ
De Mauro, G
Neto, JRTD
De Mitri, I
De Oliveira, J
de Souza, V
Debatin, J
Deligny, O
Di Giulio, C
Di Matteo, A
Castro, MLD
Diogo, F
Dobrigkeit, C
D'Olivo, JC
Dorofeev, A
dos Anjos, RC
Dova, MT
Dundovic, A
Ebr, J
Engel, R
Erdmann, M
Erfani, M
Escobar, CO
Espadanal, J
Etchegoyen, A
Falcke, H
Fang, K
Farrar, G
Fauth, AC
Fazzini, N
Fick, B
Figueira, JM
Filipcic, A
Fratu, O
Freire, MM
Fujii, T
Fuster, A
Gaior, R
Garcia, B
Garcia-Pinto, D
Gate, F
Gemmeke, H
Gherghel-Lascu, A
Ghia, PL
Giaccari, U
Giammarchi, M
Giller, M
Glas, D
Glaser, C
Glass, H
Golup, G
Berisso, MG
Vitale, PFG
Gonzalez, N
Gookin, B
Gorgi, A
Gorham, P
Gouffon, P
Grillo, AF
Grubb, TD
Guarino, F
Guedes, GP
Hampel, MR
Hansen, P
Harari, D
Harrison, TA
Harton, JL
Hasankiadeh, Q
Haungs, A
Hebbeker, T
Heck, D
Heimann, P
Herve, AE
Hill, GC
Hojvat, C
Holt, E
Homola, P
Horandel, JR
Horvath, P
Hrabovsky, M
Huege, T
Hulsman, J
Insolia, A
Isar, PG
Jandt, I
Jansen, S
Johnsen, JA
Josebachuili, M
Kaapa, A
Kambeitz, O
Kampert, KH
Kasper, P
Katkov, I
Keilhauer, B
Kemp, E
Kemp, J
Kieckhafer, RM
Klages, HO
Kleifges, M
Kleinfeller, J
Krause, R
Krohm, N
Kuempel, D
Mezek, GK
Kunka, N
Awad, AK
LaHurd, D
Lauscher, M
Lebrun, P
Legumina, R
de Oliveira, MAL
Letessier-Selvon, A
Lhenry-Yvon, I
Link, K
Lopes, L
Lopez, R
Casado, AL
Luce, Q
Lucero, A
Malacari, M
Mallamaci, M
Mandat, D
Mantsch, P
Mariazzi, AG
Maris, IC
Marsella, G
Martello, D
Martinez, H
Bravo, OM
Meza, JJM
Mathes, HJ
Mathys, S
Matthews, J
Matthews, JAJ
Matthiae, G
Mayotte, E
Mazur, PO
Medina, C
Medina-Tanco, G
Melo, D
Menshikov, A
Messina, S
Micheletti, MI
Middendorf, L
Minaya, IA
Miramonti, L
Mitrica, B
Mockler, D
Molina-Bueno, L
Mollerach, S
Montanet, F
Morello, C
Mostafa, M
Muller, G
Muller, MA
Muller, S
Naranjo, I
Nellen, L
Neuser, J
Nguyen, PH
Niculescu-Oglinzanu, M
Niechciol, M
Niemietz, L
Niggemann, T
Nitz, D
Nosek, D
Novotny, V
Nozka, H
Nunez, LA
Ochilo, L
Oikonomou, F
Olinto, A
Selmi-Dei, DP
Palatka, M
Pallotta, J
Papenbreer, P
Parente, G
Parra, A
Paul, T
Pech, M
Pedreira, F
Kala, JP
Pelayo, R
Pena-Rodriguez, J
Pereira, LAS
Perrone, L
Peters, C
Petrera, S
Phuntsok, J
Piegaia, R
Pierog, T
Pieroni, P
Pimenta, M
Pirronello, V
Platino, M
Plum, M
Porowski, C
Prado, RR
Privitera, P
Prouza, M
Quel, EJ
Querchfeld, S
Quinn, S
Ramos-Pollan, R
Rautenberg, J
Ravignani, D
Reinert, D
Revenu, B
Ridky, J
Risse, M
Ristori, P
Rizi, V
de Carvalho, WR
Fernandez, GR
Rojo, JR
Rogozin, D
Roth, M
Roulet, E
Rovero, AC
Saffi, SJ
Saftoiu, A
Salamida, F
Salazar, H
Saleh, A
Greus, FS
Salina, G
Gomez, JDS
Sanchez, F
Sanchez-Lucas, P
Santos, EM
Santos, E
Sarazin, F
Sarkar, B
Sarmento, R
Sarmiento, CA
Sato, R
Schauer, M
Scherini, V
Schieler, H
Schimp, M
Schmidt, D
Scholten, O
Schovanek, P
Schroder, FG
Schulz, A
Schulz, J
Schumacher, J
Sciutto, SJ
Segreto, A
Settimo, M
Shadkam, A
Shellard, RC
Sigl, G
Silli, G
Sima, O
Smialkowski, A
Smida, R
Snow, GR
Sommers, P
Sonntag, S
Sorokin, J
Squartini, R
Stanca, D
Stanic, S
Stasielak, J
Stassi, P
Strafella, F
Suarez, F
Duran, MS
Sudholz, T
Suomijarvi, T
Supanitsky, AD
Swain, J
Szadkowski, Z
Taboada, A
Taborda, OA
Tapia, A
Theodoro, VM
Timmermans, C
Peixoto, CJT
Tomankova, L
Tome, B
Elipe, GT
Machado, DT
Torri, M
Travnicek, P
Trini, M
Ulrich, R
Unger, M
Urban, M
Galicia, JFV
Valino, I
Valore, L
van Aar, G
van Bodegom, P
van den Berg, AM
van Vliet, A
Varela, E
Cardenas, BV
Varner, G
Vazquez, JR
Vazquez, RA
Veberic, D
Quispe, IDV
Verzi, V
Vicha, J
Villasenor, L
Vorobiov, S
Wahlberg, H
Wainberg, O
Walz, D
Watson, AA
Weber, M
Weindl, A
Wiencke, L
Wilczynski, H
Winchen, T
Wittkowski, D
Wundheiler, B
Wykes, S
Yang, L
Yelos, D
Yushkov, A
Zas, E
Zavrtanik, D
Zavrtanik, M
Zepeda, A
Zimmermann, B
Ziolkowski, M
Zong, Z
Zuccarello, F
AF Aab, A.
Abreu, P.
Aglietta, M.
Al Samarai, I.
Albuquerque, I. F. M.
Allekotte, I.
Almela, A.
Alvarez Castillo, J.
Alvarez-Muniz, J.
Ambrosio, M.
Anastasi, G. A.
Anchordoqui, L.
Andrada, B.
Andringa, S.
Aramo, C.
Arqueros, F.
Arsene, N.
Asorey, H.
Assis, P.
Aublin, J.
Avila, G.
Badescu, A. M.
Balaceanu, A.
Barreira Luz, R. J.
Baus, C.
Beatty, J. J.
Becker, K. H.
Bellido, J. A.
Berat, C.
Bertaina, E.
Bertou, X.
Biermann, P. L.
Billoir, P.
Biteau, J.
Blaess, S. G.
Blanco, A.
Blazek, J.
Bleve, C.
Bohacova, M.
Boncioli, D.
Bonifazi, C.
Borodai, N.
Botti, A. M.
Brack, J.
Brancus, I.
Bretz, T.
Bridgeman, A.
Briechle, F. L.
Buchholz, P.
Bueno, A.
Buitink, S.
Buscemi, M.
Caballero-Mora, K. S.
Caccianiga, L.
Cancio, A.
Canfora, F.
Caramete, L.
Caruso, R.
Castellina, A.
Cataldi, G.
Cazon, L.
Cester, R.
Chavez, A. G.
Chinellato, J. A.
Chudoba, J.
Clay, R. W.
Colalillo, R.
Coleman, A.
Collica, L.
Coluccia, M. R.
Conceicao, R.
Contreras, F.
Cooper, M. J.
Coutu, S.
Covault, C. E.
Cronin, J.
D'Amico, S.
Daniel, B.
Dasso, S.
Daumiller, K.
Dawson, B. R.
de Almeida, R. M.
de Jong, S. J.
De Mauro, G.
de Mello Neto, J. R. T.
De Mitri, I.
De Oliveira, J.
de Souza, V.
Debatin, J.
Deligny, O.
Di Giulio, C.
Di Matteo, A.
Diaz Castro, M. L.
Diogo, F.
Dobrigkeit, C.
D'Olivo, J. C.
Dorofeev, A.
dos Anjos, R. C.
Dova, M. T.
Dundovic, A.
Ebr, J.
Engel, R.
Erdmann, M.
Erfani, M.
Escobar, C. O.
Espadanal, J.
Etchegoyen, A.
Falcke, H.
Fang, K.
Farrar, G.
Fauth, A. C.
Fazzini, N.
Fick, B.
Figueira, J. M.
Filipcic, A.
Fratu, O.
Freire, M. M.
Fujii, T.
Fuster, A.
Gaior, R.
Garcia, B.
Garcia-Pinto, D.
Gate, F.
Gemmeke, H.
Gherghel-Lascu, A.
Ghia, P. L.
Giaccari, U.
Giammarchi, M.
Giller, M.
Glas, D.
Glaser, C.
Glass, H.
Golup, G.
Gomez Berisso, M.
Gomez Vitale, P. F.
Gonzalez, N.
Gookin, B.
Gorgi, A.
Gorham, P.
Gouffon, P.
Grillo, A. F.
Grubb, T. D.
Guarino, F.
Guedes, G. P.
Hampel, M. R.
Hansen, P.
Harari, D.
Harrison, T. A.
Harton, J. L.
Hasankiadeh, Q.
Haungs, A.
Hebbeker, T.
Heck, D.
Heimann, P.
Herve, A. E.
Hill, G. C.
Hojvat, C.
Holt, E.
Homola, P.
Horandel, J. R.
Horvath, P.
Hrabovsky, M.
Huege, T.
Hulsman, J.
Insolia, A.
Isar, P. G.
Jandt, I.
Jansen, S.
Johnsen, J. A.
Josebachuili, M.
Kaeaepae, A.
Kambeitz, O.
Kampert, K. H.
Kasper, P.
Katkov, I.
Keilhauer, B.
Kemp, E.
Kemp, J.
Kieckhafer, R. M.
Klages, H. O.
Kleifges, M.
Kleinfeller, J.
Krause, R.
Krohm, N.
Kuempel, D.
Mezek, G. Kukec
Kunka, N.
Awad, A. Kuotb
LaHurd, D.
Lauscher, M.
Lebrun, P.
Legumina, R.
Leigui de Oliveira, M. A.
Letessier-Selvon, A.
Lhenry-Yvon, I.
Link, K.
Lopes, L.
Lopez, R.
Lopez Casado, A.
Luce, Q.
Lucero, A.
Malacari, M.
Mallamaci, M.
Mandat, D.
Mantsch, P.
Mariazzi, A. G.
Maris, I. C.
Marsella, G.
Martello, D.
Martinez, H.
Martinez Bravo, O.
Masias Meza, J. J.
Mathes, H. J.
Mathys, S.
Matthews, J.
Matthews, J. A. J.
Matthiae, G.
Mayotte, E.
Mazur, P. O.
Medina, C.
Medina-Tanco, G.
Melo, D.
Menshikov, A.
Messina, S.
Micheletti, M. I.
Middendorf, L.
Minaya, I. A.
Miramonti, L.
Mitrica, B.
Mockler, D.
Molina-Bueno, L.
Mollerach, S.
Montanet, F.
Morello, C.
Mostafa, M.
Mueller, G.
Muller, M. A.
Mueller, S.
Naranjo, I.
Nellen, L.
Neuser, J.
Nguyen, P. H.
Niculescu-Oglinzanu, M.
Niechciol, M.
Niemietz, L.
Niggemann, T.
Nitz, D.
Nosek, D.
Novotny, V.
Nozka, H.
Nunez, L. A.
Ochilo, L.
Oikonomou, F.
Olinto, A.
Pakk Selmi-Dei, D.
Palatka, M.
Pallotta, J.
Papenbreer, P.
Parente, G.
Parra, A.
Paul, T.
Pech, M.
Pedreira, F.
Kala, J. Pe
Pelayo, R.
Pena-Rodriguez, J.
Pereira, L. A. S.
Perrone, L.
Peters, C.
Petrera, S.
Phuntsok, J.
Piegaia, R.
Pierog, T.
Pieroni, P.
Pimenta, M.
Pirronello, V.
Platino, M.
Plum, M.
Porowski, C.
Prado, R. R.
Privitera, P.
Prouza, M.
Quel, E. J.
Querchfeld, S.
Quinn, S.
Ramos-Pollan, R.
Rautenberg, J.
Ravignani, D.
Reinert, D.
Revenu, B.
Ridky, J.
Risse, M.
Ristori, P.
Rizi, V.
Rodrigues de Carvalho, W.
Fernandez, G. Rodriguez
Rodriguez Rojo, J.
Rogozin, D.
Roth, M.
Roulet, E.
Rovero, A. C.
Saffi, S. J.
Saftoiu, A.
Salamida, F.
Salazar, H.
Saleh, A.
Greus, F. Salesa
Salina, G.
Sanabria Gomez, J. D.
Sanchez, F.
Sanchez-Lucas, P.
Santos, E. M.
Santos, E.
Sarazin, F.
Sarkar, B.
Sarmento, R.
Sarmiento, C. A.
Sato, R.
Schauer, M.
Scherini, V.
Schieler, H.
Schimp, M.
Schmidt, D.
Scholten, O.
Schovanek, P.
Schroder, F. G.
Schulz, A.
Schulz, J.
Schumacher, J.
Sciutto, S. J.
Segreto, A.
Settimo, M.
Shadkam, A.
Shellard, R. C.
Sigl, G.
Silli, G.
Sima, O.
Smialkowski, A.
Smida, R.
Snow, G. R.
Sommers, P.
Sonntag, S.
Sorokin, J.
Squartini, R.
Stanca, D.
Stanic, S.
Stasielak, J.
Stassi, P.
Strafella, F.
Suarez, F.
Suarez Duran, M.
Sudholz, T.
Suomijarvi, T.
Supanitsky, A. D.
Swain, J.
Szadkowski, Z.
Taboada, A.
Taborda, O. A.
Tapia, A.
Theodoro, V. M.
Timmermans, C.
Todero Peixoto, C. J.
Tomankova, L.
Tome, B.
Torralba Elipe, G.
Torres Machado, D.
Torri, M.
Travnicek, P.
Trini, M.
Ulrich, R.
Unger, M.
Urban, M.
Valdes Galicia, J. F.
Valino, I.
Valore, L.
van Aar, G.
van Bodegom, P.
van den Berg, A. M.
van Vliet, A.
Varela, E.
Vargas Cardenas, B.
Varner, G.
Vazquez, J. R.
Vazquez, R. A.
Veberic, D.
Vergara Quispe, I. D.
Verzi, V.
Vicha, J.
Villasenor, L.
Vorobiov, S.
Wahlberg, H.
Wainberg, O.
Walz, D.
Watson, A. A.
Weber, M.
Weindl, A.
Wiencke, L.
Wilczynski, H.
Winchen, T.
Wittkowski, D.
Wundheiler, B.
Wykes, S.
Yang, L.
Yelos, D.
Yushkov, A.
Zas, E.
Zavrtanik, D.
Zavrtanik, M.
Zepeda, A.
Zimmermann, B.
Ziolkowski, M.
Zong, Z.
Zuccarello, F.
CA Pierre Auger Collaboration
TI Search for ultrarelativistic magnetic monopoles with the Pierre Auger
observatory
SO PHYSICAL REVIEW D
LA English
DT Article
ID FLUORESCENCE YIELD; ENERGY-LOSS; DETECTOR; FLUX
AB We present a search for ultrarelativistic magnetic monopoles with the Pierre Auger observatory. Such particles, possibly a relic of phase transitions in the early Universe, would deposit a large amount of energy along their path through the atmosphere, comparable to that of ultrahigh-energy cosmic rays (UHECRs). The air-shower profile of a magnetic monopole can be effectively distinguished by the fluorescence detector from that of standard UHECRs. No candidate was found in the data collected between 2004 and 2012, with an expected background of less than 0.1 event from UHECRs. The corresponding 90% confidence level (C.L.) upper limits on the flux of ultrarelativistic magnetic monopoles range from 10(-1)9 (cm(2) sr s)(-1) for a Lorentz factor gamma = 10(9) to 2.5 x 10(-21) (cm(2) sr s)(-1) for gamma = 10(12). These results-the first obtained with a UHECR detector-improve previously published limits by up to an order of magnitude.
C1 [Aab, A.; Buchholz, P.; Erfani, M.; Heimann, P.; Niechciol, M.; Ochilo, L.; Risse, M.; Sonntag, S.; Ziolkowski, M.] Univ Siegen, Fachbereich Phys Expt Teilchenphys 7, D-57068 Siegen, Germany.
[Abreu, P.; Andringa, S.; Assis, P.; Barreira Luz, R. J.; Blanco, A.; Cazon, L.; Conceicao, R.; Diogo, F.; Espadanal, J.; Lopes, L.; Pimenta, M.; Sarmento, R.; Tome, B.] UL, Lab Instrumentacao & Fis Expt Particulas LIP, Lisbon, Portugal.
[Abreu, P.; Andringa, S.; Assis, P.; Barreira Luz, R. J.; Blanco, A.; Cazon, L.; Conceicao, R.; Diogo, F.; Espadanal, J.; Lopes, L.; Pimenta, M.; Sarmento, R.; Tome, B.] UL, IST, Lisbon, Portugal.
[Aglietta, M.; Castellina, A.; Gorgi, A.; Morello, C.] INAF, Osservatorio Astrofis Torino, Turin, Italy.
[Aglietta, M.; Bertaina, E.; Castellina, A.; Cester, R.; Collica, L.; Gorgi, A.; Morello, C.] Ist Nazl Fis Nucl, Sez Torino, Turin, Italy.
[Al Samarai, I.; Aublin, J.; Billoir, P.; Caccianiga, L.; Gaior, R.; Letessier-Selvon, A.; Settimo, M.] Univ Paris 06, LPNHE, F-75252 Paris 05, France.
[Al Samarai, I.; Aublin, J.; Billoir, P.; Caccianiga, L.; Gaior, R.; Letessier-Selvon, A.; Settimo, M.] Univ Paris 07, CNRS IN2P3, F-75252 Paris 05, France.
[Albuquerque, I. F. M.; Gouffon, P.; Rodrigues de Carvalho, W.; Santos, E. M.] Univ Sao Paulo, Inst Fis, Sao Paulo, Brazil.
[Allekotte, I.; Asorey, H.; Bertou, X.; Golup, G.; Gomez Berisso, M.; Harari, D.; Mollerach, S.; Naranjo, I.; Roulet, E.; Taborda, O. A.] Consejo Nacl Invest Cient & Tecn, Ctr Atom Bariloche, RA-1033 Buenos Aires, DF, Argentina.
[Allekotte, I.; Asorey, H.; Bertou, X.; Golup, G.; Gomez Berisso, M.; Harari, D.; Mollerach, S.; Naranjo, I.; Roulet, E.; Taborda, O. A.] Consejo Nacl Invest Cient & Tecn, UNCuyo, CNEA, Inst Balseiro, RA-1033 Buenos Aires, DF, Argentina.
[Almela, A.; Andrada, B.; Botti, A. M.; Etchegoyen, A.; Figueira, J. M.; Fuster, A.; Gonzalez, N.; Hampel, M. R.; Holt, E.; Hulsman, J.; Josebachuili, M.; Lucero, A.; Melo, D.; Mueller, S.; Platino, M.; Ravignani, D.; Sanchez, F.; Santos, E.; Sarmiento, C. A.; Schmidt, D.; Silli, G.; Suarez, F.; Tapia, A.; Wainberg, O.; Wundheiler, B.; Yelos, D.; Yushkov, A.] Consejo Nacl Invest Cient & Tecn, UNSAM, Ctr Atom Constituyentes, Comis Nacl Energia Atom,CNEA,Inst Tecnol Detecc &, RA-1033 Buenos Aires, DF, Argentina.
Univ Tecnol Nacl, Fac Reg Buenos Aires, Buenos Aires, DF, Argentina.
[Alvarez Castillo, J.; D'Olivo, J. C.; Medina-Tanco, G.; Nellen, L.; Valdes Galicia, J. F.; Vargas Cardenas, B.] Univ Nacl Autonoma Mexico, Buenos Aires, DF, Argentina.
[Alvarez-Muniz, J.; Lopez Casado, A.; Parente, G.; Pedreira, F.; Torralba Elipe, G.; Valino, I.; Vazquez, R. A.; Zas, E.] Univ Santiago de Compostela, Santiago De Compostela, Spain.
[Ambrosio, M.; Aramo, C.; Colalillo, R.; Guarino, F.; Valore, L.] Ist Nazl Fis Nucl, Sez Napoli, Milan, Italy.
[Anastasi, G. A.; Petrera, S.] Ist Nazl Fis Nucl, Gran Sasso Sci Inst, Laquila, Italy.
[Anchordoqui, L.; Paul, T.] CUNY, Lehman Coll, Dept Phys & Astron, New York, NY USA.
[Arqueros, F.; Garcia-Pinto, D.; Minaya, I. A.; Vazquez, J. R.] Univ Complutense Madrid, E-28040 Madrid, Spain.
[Arsene, N.; Sima, O.] Univ Bucharest, Dept Phys, Bucharest, Romania.
[Asorey, H.; Nunez, L. A.; Pena-Rodriguez, J.; Ramos-Pollan, R.; Sanabria Gomez, J. D.; Suarez Duran, M.] Univ Ind Santander, Santander, Colombia.
[Avila, G.; Contreras, F.; Gomez Vitale, P. F.; Kleinfeller, J.; Rodriguez Rojo, J.; Sato, R.; Squartini, R.] Observ Pierre Auger, Buenos Aires, DF, Argentina.
[Avila, G.; Contreras, F.; Gomez Vitale, P. F.] Comis Nacl Energia Atom, Buenos Aires, DF, Argentina.
[Badescu, A. M.; Fratu, O.] Univ Politehn Bucuresti, Bucharest, Romania.
[Balaceanu, A.; Brancus, I.; Gherghel-Lascu, A.; Mitrica, B.; Niculescu-Oglinzanu, M.; Saftoiu, A.; Stanca, D.] Horia Hulubei Natl Inst Phys & Nucl Engn, Bucharest 077125, Romania.
[Baus, C.; Herve, A. E.; Kambeitz, O.; Katkov, I.; Link, K.; Mockler, D.; Taboada, A.] Karlsruhe Inst Technol, Inst Expt Kernphys IEKP, D-76021 Karlsruhe, Germany.
[Beatty, J. J.] Ohio State Univ, Columbus, OH 43210 USA.
[Becker, K. H.; Jandt, I.; Kaeaepae, A.; Kampert, K. H.; Krohm, N.; Mathys, S.; Mayotte, E.; Neuser, J.; Niemietz, L.; Papenbreer, P.; Querchfeld, S.; Rautenberg, J.; Sarkar, B.; Schauer, M.; Schimp, M.; Winchen, T.; Wittkowski, D.] Univ Wuppertal, Dept Phys, Wuppertal, Germany.
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[Giammarchi, M.; Mallamaci, M.; Miramonti, L.] Ist Nazl Fis Nucl, Sez Milano, Milan, Italy.
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[Salamida, F.] Ist Nazl Fis Nucl, Sez Milano Bicocca, Milan, Italy.
[Scholten, O.] Vrije Univ Brussels, Brussels, Belgium.
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[Watson, A. A.] Univ Leeds, Sch Phys & Astron, Leeds, W Yorkshire, England.
RP Aab, A (reprint author), Univ Siegen, Fachbereich Phys Expt Teilchenphys 7, D-57068 Siegen, Germany.
EM auger_spokespersons@fnal.gov
RI Valino, Ines/J-8324-2012; Arqueros, Fernando/K-9460-2014; Horvath,
Pavel/G-6334-2014; De Mitri, Ivan/C-1728-2017; Mitrica,
Bogdan/D-5201-2009; Alvarez-Muniz, Jaime/H-1857-2015; Bueno,
Antonio/F-3875-2015; dos Santos, Eva/N-6351-2013; Rodriguez Fernandez,
Gonzalo/C-1432-2014; Nosek, Dalibor/F-1129-2017; Buscemi,
Mario/R-5071-2016; Colalillo, Roberta/R-5088-2016; de Mello Neto,
Joao/C-5822-2013; de souza, Vitor/D-1381-2012; Badescu,
Alina/B-6087-2012; Sao Carlos Institute of Physics,
IFSC/USP/M-2664-2016; Chinellato, Carola Dobrigkeit /F-2540-2011;
Beatty, James/D-9310-2011; Caramete, Laurentiu/C-2328-2011; Assis,
Pedro/D-9062-2013; Guarino, Fausto/I-3166-2012; Zuccarello,
Francesca/R-1834-2016;
OI Valino, Ines/0000-0001-7823-0154; Arqueros,
Fernando/0000-0002-4930-9282; Horvath, Pavel/0000-0002-6710-5339; De
Mitri, Ivan/0000-0002-8665-1730; Alvarez-Muniz,
Jaime/0000-0002-2367-0803; Bueno, Antonio/0000-0002-7439-4247; dos
Santos, Eva/0000-0002-0474-8863; Rodriguez Fernandez,
Gonzalo/0000-0002-4683-230X; Nosek, Dalibor/0000-0001-6219-200X;
Buscemi, Mario/0000-0003-2123-5434; Colalillo,
Roberta/0000-0002-4179-9352; de Mello Neto, Joao/0000-0002-3234-6634;
Chinellato, Carola Dobrigkeit /0000-0002-1236-0789; Beatty,
James/0000-0003-0481-4952; Assis, Pedro/0000-0001-7765-3606; Guarino,
Fausto/0000-0003-1427-9885; Zuccarello, Francesca/0000-0003-1853-2550;
Novotny, Vladimir/0000-0002-4319-4541; Garcia,
Beatriz/0000-0003-0919-2734; Nunez, Luis/0000-0003-4575-5899; Coutu,
Stephane/0000-0003-2923-2246
FU Comision Nacional de Energia Atomica; Agencia Nacional de Promocion
Cientifica y Tecnologica (ANPCyT); Consejo Nacional de Investigaciones
Cientificas y Tecnicas (CONICET); Australian Research Council; Conselho
Nacional de Desenvolvimento Cientifico e Tecnologico (CNPq);
Financiadora de Estudos e Projetos (FINEP); Fundacao de Amparo a
Pesquisa do Estado de Rio de Janeiro (FAPERJ); Sao Paulo Research
Foundation (FAPESP) [2010/07359-6, 1999/05404-3]; Gobierno de la
Provincia de Mendoza, Argentina; Municipalidad de Malargue, Argentina;
NDM Holdings, Argentina; Valle Las Lenas, Argentina; Ministerio de
Ciencia e Tecnologia (MCT), Brazil [MSMT CR LG15014, LO1305, LM2015038];
Czech Science Foundation, Czech Republic [14-17501S]; Centre de Calcul
IN2P3/CNRS, France; Centre National de la Recherche Scientifique (CNRS),
France; Conseil Regional Ile-de-France, France; Departement Physique
Nucleaire et Corpusculaire (PNC-IN2P3/CNRS), France; Departement
Sciences de l'Univers (SDU-INSU/CNRS), France; Institut Lagrange de
Paris (ILP) Grant, within the Investissements d'Avenir Programme Grant,
France [LABEX ANR-10-LABX-63, ANR-11-IDEX-0004-02]; Bundesministerium
fur Bildung und Forschung (BMBF); Deutsche Forschungsgemeinschaft (DFG);
Finanzministerium Baden-Wurttemberg; Helmholtz Alliance for
Astroparticle Physics (HAP); Helmholtz-Gemeinschaft Deutscher
Forschungszentren (HGF); Ministerium fur Wissenschaft und Forschung,
Nordrhein Westfalen; Ministerium fur Wissenschaft, Forschung und Kunst,
Baden-Wurttemberg, Germany; Istituto Nazionale di Fisica Nucleare
(INFN); Istituto Nazionale di Astrofisica (INAF); Ministero
dell'Istruzione, dell'Universita e della Ricerca (MIUR); Gran Sasso
Center for Astroparticle Physics (CFA); CETEMPS Center of Excellence;
Ministero degli Affari Esteri (MAE), Italy; Consejo Nacional de Ciencia
y Tecnologia (CONACYT), Mexico [167733]; Universidad Nacional Autonoma
de Mexico (UNAM), PAPIIT DGAPA-UNAM, Mexico; Ministerie van Onderwijs,
Cultuur en Wetenschap; Nederlandse Organisatie voor Wetenschappelijk
Onderzoek (NWO); Stichting voor Fundamenteel Onderzoek der Materie
(FOM), Netherlands; National Centre for Research and Development
[ERA-NET-ASPERA/01/11, ERA-NET-ASPERA/02/11]; National Science Centre,
Poland [2013/08/M/ST9/00322, 2013/08/M/ST9/00728, HARMONIA
5-2013/10/M/ST9/00062]; Portuguese national funds; FEDER funds within
Programa Operacional Factores de Competitividade through Fundacao para a
Ciencia e a Tecnologia (COMPETE), Portugal; Romanian Authority for
Scientific Research ANCS, CNDI-UEFISCDI partnership projects [20/2012,
194/2012, PN 16 42 01 02]; Slovenian Research Agency, Slovenia;
Comunidad de Madrid, Fondo Europeo de Desarrollo Regional (FEDER) funds;
Ministerio de Economia y Competitividad; Xunta de Galicia; European
Community 7th Framework Program, Spain [FP7-PEOPLE-2012-IEF-328826];
Science and Technology Facilities Council, United Kingdom; Department of
Energy [DE-AC02-07CH11359, DE-FR02-04ER41300, DE-FG02-99ER41107,
DE-SC0011689]; National Science Foundation [0450696]; Grainger
Foundation, USA; NAFOSTED, Vietnam; Marie Curie-IRSES/EPLANET, European
Particle Physics Latin American Network, European Union 7th Framework
Program [PIRSES-2009-GA-246806]; UNESCO; NSF [PHY-1412261]; Kavli
Institute for Cosmological Physics at the University of Chicago [NSF
PHY-1125897]; Japan Society for the Promotion of Science [H25-339]
FX The successful installation, commissioning, and operation of the Pierre
Auger observatory would not have been possible without the strong
commitment and effort from the technical and administrative staff in
Malargue. We are very grateful to the following agencies and
organizations for financial support: Comision Nacional de Energia
Atomica, Agencia Nacional de Promocion Cientifica y Tecnologica
(ANPCyT), Consejo Nacional de Investigaciones Cientificas y Tecnicas
(CONICET), and Gobierno de la Provincia de Mendoza, Municipalidad de
Malargue, NDM Holdings and Valle Las Lenas, Argentina, in gratitude for
their continuing cooperation over land access; the Australian Research
Council; Conselho Nacional de Desenvolvimento Cientifico e Tecnologico
(CNPq), Financiadora de Estudos e Projetos (FINEP), Fundacao de Amparo a
Pesquisa do Estado de Rio de Janeiro (FAPERJ), Sao Paulo Research
Foundation (FAPESP) Grants No. 2010/07359-6 and No. 1999/05404-3,
Ministerio de Ciencia e Tecnologia (MCT), Brazil, Grants No. MSMT CR
LG15014, No. LO1305 and No. LM2015038 and the Czech Science Foundation
Grant No. 14-17501S, Czech Republic; Centre de Calcul IN2P3/CNRS, Centre
National de la Recherche Scientifique (CNRS), Conseil Regional
Ile-de-France, Departement Physique Nucleaire et Corpusculaire
(PNC-IN2P3/CNRS), Departement Sciences de l'Univers (SDU-INSU/CNRS), and
Institut Lagrange de Paris (ILP) Grant No. LABEX ANR-10-LABX-63, within
the Investissements d'Avenir Programme Grant No. ANR-11-IDEX-0004-02,
France; Bundesministerium fur Bildung und Forschung (BMBF), Deutsche
Forschungsgemeinschaft (DFG), Finanzministerium Baden-Wurttemberg,
Helmholtz Alliance for Astroparticle Physics (HAP),
Helmholtz-Gemeinschaft Deutscher Forschungszentren (HGF), Ministerium
fur Wissenschaft und Forschung, Nordrhein Westfalen, Ministerium fur
Wissenschaft, Forschung und Kunst, Baden-Wurttemberg, Germany; Istituto
Nazionale di Fisica Nucleare (INFN), Istituto Nazionale di Astrofisica
(INAF), Ministero dell'Istruzione, dell'Universita e della Ricerca
(MIUR), Gran Sasso Center for Astroparticle Physics (CFA), CETEMPS
Center of Excellence, and Ministero degli Affari Esteri (MAE), Italy;
Consejo Nacional de Ciencia y Tecnologia (CONACYT) Grant No. 167733,
Mexico; Universidad Nacional Autonoma de Mexico (UNAM), PAPIIT
DGAPA-UNAM, Mexico; Ministerie van Onderwijs, Cultuur en Wetenschap,
Nederlandse Organisatie voor Wetenschappelijk Onderzoek (NWO), and
Stichting voor Fundamenteel Onderzoek der Materie (FOM), Netherlands;
National Centre for Research and Development, Grants No.
ERA-NET-ASPERA/01/11 and No. ERA-NET-ASPERA/02/11, and National Science
Centre, Grants No. 2013/08/M/ST9/00322, No. 2013/08/M/ST9/00728 and No.
HARMONIA 5-2013/10/M/ST9/00062, Poland; Portuguese national funds and
FEDER funds within Programa Operacional Factores de Competitividade
through Fundacao para a Ciencia e a Tecnologia (COMPETE), Portugal;
Romanian Authority for Scientific Research ANCS, CNDI-UEFISCDI
partnership projects Grants No. 20/2012, No. 194/2012 and No. PN 16 42
01 02; Slovenian Research Agency, Slovenia; Comunidad de Madrid, Fondo
Europeo de Desarrollo Regional (FEDER) funds, Ministerio de Economia y
Competitividad, Xunta de Galicia, and European Community 7th Framework
Program, Grant No. FP7-PEOPLE-2012-IEF-328826, Spain; Science and
Technology Facilities Council, United Kingdom; Department of Energy
Awards No. DE-AC02-07CH11359, No. DE-FR02-04ER41300, No.
DE-FG02-99ER41107 and No. DE-SC0011689, National Science Foundation,
Grant No.; 0450696, and The Grainger Foundation, USA; NAFOSTED, Vietnam;
Marie Curie-IRSES/EPLANET, European Particle Physics Latin American
Network, European Union 7th Framework Program, Grant No.
PIRSES-2009-GA-246806; and UNESCO. This work was supported in part by
NSF Grant No. PHY-1412261 and by the Kavli Institute for Cosmological
Physics at the University of Chicago through Grant No. NSF PHY-1125897
and an endowment from the Kavli Foundation and its founder Fred Kavli.
T. F. was supported by the Japan Society for the Promotion of Science
Fellowship for Research Abroad Grant No. H25-339.
NR 39
TC 0
Z9 0
U1 46
U2 46
PU AMER PHYSICAL SOC
PI COLLEGE PK
PA ONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA
SN 2470-0010
EI 2470-0029
J9 PHYS REV D
JI Phys. Rev. D
PD OCT 3
PY 2016
VL 94
IS 8
AR 082002
DI 10.1103/PhysRevD.94.082002
PG 12
WC Astronomy & Astrophysics; Physics, Particles & Fields
SC Astronomy & Astrophysics; Physics
GA DX6DZ
UT WOS:000384474700002
ER
PT J
AU Hoskins, J
Crisosto, N
Gleason, J
Sikivie, P
Stern, I
Sullivan, NS
Tanner, DB
Boutan, C
Hotz, M
Khatiwada, R
Lyapustin, D
Malagon, A
Ottens, R
Rosenberg, LJ
Rybka, G
Sloan, J
Wagner, A
Will, D
Carosi, G
Carter, D
Duffy, LD
Bradley, R
Clarke, J
O'Kelley, S
van Bibber, K
Daw, EJ
AF Hoskins, J.
Crisosto, N.
Gleason, J.
Sikivie, P.
Stern, I.
Sullivan, N. S.
Tanner, D. B.
Boutan, C.
Hotz, M.
Khatiwada, R.
Lyapustin, D.
Malagon, A.
Ottens, R.
Rosenberg, L. J.
Rybka, G.
Sloan, J.
Wagner, A.
Will, D.
Carosi, G.
Carter, D.
Duffy, L. D.
Bradley, R.
Clarke, J.
O'Kelley, S.
van Bibber, K.
Daw, E. J.
TI Modulation sensitive search for nonvirialized dark-matter axions
SO PHYSICAL REVIEW D
LA English
DT Article
ID INVISIBLE-AXION; CP CONSERVATION; HARMLESS AXION; COSMIC AXIONS;
INVARIANCE; PARTICLES; DENSITY
AB Nonvirialized dark-matter axions may be present in the Milky Way halo in the form of low-velocity-dispersion flows. The Axion Dark-Matter eXperiment performed a search for the conversion of these axions into microwave photons using a resonant cavity immersed in a strong, static magnetic field. The spread of photon energy in these measurements was measured at spectral resolutions of the order of 1 Hz and below. If the energy variation were this small, the frequency modulation of any real axion signal due to the orbital and rotational motion of Earth would become non-negligible. Conservative estimates of the expected signal modulation were made and used as a guide for the search procedure. The photon frequencies covered by this search are 812-852 and 858-892 MHz, which correspond to an axion mass of 3.36-3.52 and 3.55-3.69 mu eV. No axion signal was found, and limits were placed on the maximum local density of nonvirialized axions of these masses.
C1 [Hoskins, J.; Crisosto, N.; Gleason, J.; Sikivie, P.; Stern, I.; Sullivan, N. S.; Tanner, D. B.] Univ Florida, Gainesville, FL 32611 USA.
[Boutan, C.; Hotz, M.; Khatiwada, R.; Lyapustin, D.; Malagon, A.; Ottens, R.; Rosenberg, L. J.; Rybka, G.; Sloan, J.; Wagner, A.; Will, D.] Univ Washington, Seattle, WA 98195 USA.
[Carosi, G.; Carter, D.] Lawrence Livermore Natl Lab, Livermore, CA 94550 USA.
[Duffy, L. D.] Los Alamos Natl Lab, Los Alamos, NM 87544 USA.
[Bradley, R.] Natl Radio Astron Observ, Charlottesville, VA 22903 USA.
[Clarke, J.; O'Kelley, S.; van Bibber, K.] Univ Calif Berkeley, Berkeley, CA 94720 USA.
[Daw, E. J.] Univ Sheffield, Western Bank, Sheffield S10 2TN, S Yorkshire, England.
[Wagner, A.] Raytheon BBN Technol, Quantum Informat Div, 10 Moulton St, Cambridge, MA 02138 USA.
RP Hoskins, J (reprint author), Univ Florida, Gainesville, FL 32611 USA.
OI Stern, Ian/0000-0002-1166-465X
FU U.S. Department of Energy [DE-SC0010280, DE-FG02-97ER41029,
DE-FG02-96ER40956, DE-AC52-07NA27344, DE-AC03-76SF00098]; Heising-Simons
Foundation; Lawrence Livermore National Laboratory LDRD program
FX This work was supported by the U.S. Department of Energy through Grants
No. DE-SC0010280, No. DE-FG02-97ER41029, No. DE-FG02-96ER40956, No.
DE-AC52-07NA27344, and No. DE-AC03-76SF00098. Additional support was
provided by the Heising-Simons Foundation and the Lawrence Livermore
National Laboratory LDRD program.
NR 31
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PU AMER PHYSICAL SOC
PI COLLEGE PK
PA ONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA
SN 2470-0010
EI 2470-0029
J9 PHYS REV D
JI Phys. Rev. D
PD OCT 3
PY 2016
VL 94
IS 8
AR 082001
DI 10.1103/PhysRevD.94.082001
PG 13
WC Astronomy & Astrophysics; Physics, Particles & Fields
SC Astronomy & Astrophysics; Physics
GA DX6DZ
UT WOS:000384474700001
ER
PT J
AU Mrenna, S
Skands, P
AF Mrenna, S.
Skands, P.
TI Automated parton- shower variations in PYTHIA 8
SO PHYSICAL REVIEW D
LA English
DT Article
ID SUDAKOV VETO ALGORITHM; EVENT STRUCTURE; QCD CASCADES; SCATTERING;
SIMULATION; AMPLITUDES; MODEL
AB In the era of precision physics measurements at the LHC, efficient and exhaustive estimations of theoretical uncertainties play an increasingly crucial role. In the context of Monte Carlo (MC) event generators, the estimation of such uncertainties traditionally requires independent MC runs for each variation, for a linear increase in total run time. In this work, we report on an automated evaluation of the dominant (renormalization-scale and nonsingular) perturbative uncertainties in the PYTHIA 8 event generator, with only a modest computational overhead. Each generated event is accompanied by a vector of alternative weights (one for each uncertainty variation), with each set separately preserving the total cross section. Explicit scale-compensating terms can be included, reflecting known coefficients of higher-order splitting terms and reducing the effect of the variations. The formalism also allows for the enhancement of rare partonic splittings, such as g -> bb and q -> q gamma, to obtain weighted samples enriched in these splittings while preserving the correct physical Sudakov factors.
C1 [Mrenna, S.] Fermilab Natl Accelerator Lab, Comp Div, Batavia, IL 60510 USA.
[Skands, P.] Monash Univ, Sch Phys & Astron, Melbourne, Vic 3800, Australia.
RP Mrenna, S (reprint author), Fermilab Natl Accelerator Lab, Comp Div, Batavia, IL 60510 USA.
OI Skands, Peter/0000-0003-0024-3822
FU Australian Research Council [FT130100744]; U.S. Department of Energy
[DE-AC02-07CH11359]
FX The motivation to undertake this work arose from discussions at the
Physics at TeV Colliders Workshop, Les Houches, June 2015. P.S. is
supported in part by the Australian Research Council, Contract No.
FT130100744. Fermilab is operated by the Fermi Research Alliance, LLC
under Contract No. DE-AC02-07CH11359 with the U.S. Department of Energy.
NR 42
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PU AMER PHYSICAL SOC
PI COLLEGE PK
PA ONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA
SN 2470-0010
EI 2470-0029
J9 PHYS REV D
JI Phys. Rev. D
PD OCT 3
PY 2016
VL 94
IS 7
AR 074005
DI 10.1103/PhysRevD.94.074005
PG 14
WC Astronomy & Astrophysics; Physics, Particles & Fields
SC Astronomy & Astrophysics; Physics
GA DX6DO
UT WOS:000384473600005
ER
PT J
AU Brajuskovic, V
Barrows, F
Phatak, C
Petford-Long, AK
AF Brajuskovic, V.
Barrows, F.
Phatak, C.
Petford-Long, A. K.
TI Real-space observation of magnetic excitations and avalanche behavior in
artificial quasicrystal lattices
SO SCIENTIFIC REPORTS
LA English
DT Article
ID SPIN-ICE
AB Artificial spin ice lattices have emerged as model systems for studying magnetic frustration in recent years. Most work to date has looked at periodic artificial spin ice lattices. In this paper, we observe frustration effects in quasicrystal artificial spin ice lattices that lack translational symmetry and contain vertices with different numbers of interacting elements. We find that as the lattice state changes following demagnetizing and annealing, specific vertex motifs retain low-energy configurations, which excites other motifs into higher energy configurations. Additionally, we find that unlike the magnetization reversal process for periodic artificial spin ice lattices, which occurs through 1D avalanches, quasicrystal lattices undergo reversal through a dendritic 2D avalanche mechanism.
C1 [Brajuskovic, V.; Barrows, F.; Phatak, C.; Petford-Long, A. K.] Argonne Natl Lab, Div Mat Sci, 9700 S Cass Ave, Lemont, IL 60439 USA.
[Brajuskovic, V.; Petford-Long, A. K.] Northwestern Univ, Dept Mat Sci & Engn, 2220 Campus Dr, Evanston, IL 60208 USA.
[Barrows, F.] Northwestern Univ, Appl Phys Program, 2220 Campus Dr, Evanston, IL 60208 USA.
RP Phatak, C (reprint author), Argonne Natl Lab, Div Mat Sci, 9700 S Cass Ave, Lemont, IL 60439 USA.
EM cd@anl.gov
FU US Department of Energy, Office of Science, Basic Energy Sciences,
Materials Sciences and Engineering Division; US Department of Energy,
Office of Science, Office of Basic Energy Sciences [DE-AC02-06CH11357]
FX This work was supported by the US Department of Energy, Office of
Science, Basic Energy Sciences, Materials Sciences and Engineering
Division. Use of the Center for Nanoscale Materials was supported by the
US Department of Energy, Office of Science, Office of Basic Energy
Sciences, under contract no. DE-AC02-06CH11357. We acknowledge J.
Pearson for help with thin film deposition.
NR 28
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U1 8
U2 8
PU NATURE PUBLISHING GROUP
PI LONDON
PA MACMILLAN BUILDING, 4 CRINAN ST, LONDON N1 9XW, ENGLAND
SN 2045-2322
J9 SCI REP-UK
JI Sci Rep
PD OCT 3
PY 2016
VL 6
AR 34384
DI 10.1038/srep34384
PG 10
WC Multidisciplinary Sciences
SC Science & Technology - Other Topics
GA DX5MO
UT WOS:000384425300001
PM 27694973
ER
PT J
AU Sarkar, A
Milioli, FE
Ozarkar, S
Li, TW
Sun, X
Sundaresan, S
AF Sarkar, Avik
Milioli, Fernando E.
Ozarkar, Shailesh
Li, Tingwen
Sun, Xin
Sundaresan, Sankaran
TI Filtered sub-grid constitutive models for fluidized gas-particle flows
constructed from 3-D simulations
SO CHEMICAL ENGINEERING SCIENCE
LA English
DT Article
DE Computational fluid dynamics (CFD); Constitutive models; Fluidization;
Multiphase flow; Scale-up; Two-fluid model
ID TRAVELING-WAVE SOLUTIONS; 2-FLUID MODELS; CYLINDER ARRAYS; SOLID FLOWS;
DRAG MODELS; BEDS; VALIDATION; CHALLENGES; EQUATIONS; DIFFUSION
AB The accuracy of fluidized-bed CFD predictions using the two-fluid model can be improved significantly, even when using coarse grids, by replacing the microscopic kinetic-theory-based closures with coarse grained constitutive models. These coarse-grained constitutive relationships, called filtered models, account for the unresolved gas-particle structures (clusters and bubbles) via sub-grid corrections. Following the previous 2-D approaches of Igci et al. [AIChE J., 54(6), 1431-1448, 2008] and Milioli et al. [AIChE J., 59(9), 3265-3275, 2013], new closures for the filtered inter-phase drag and stresses in the gas and particle phases are constructed from highly-resolved 3-D simulations of gas-particle flows. These new closure relations are then validated through the bubbling-fluidized-bed challenge problem presented by National Energy Technology Laboratory and Particulate Solids Research Inc. (C) 2016 Elsevier Ltd. All rights reserved.
C1 [Sarkar, Avik; Sun, Xin] Pacific Northwest Natl Lab, Fundamental & Computat Sci Directorate, POB 999,MSIN K7-90, Richland, WA 99352 USA.
[Sarkar, Avik] Pfizer Inc, Worldwide Res & Dev, MS 8156-014,Eastern Point Rd, Groton, CT 06340 USA.
[Milioli, Fernando E.; Sundaresan, Sankaran] Princeton Univ, Chem & Biol Engn, A-315 Engn Quadrangle, Princeton, NJ 08544 USA.
[Ozarkar, Shailesh] ANSYS Inc, Canonsburg, PA 15317 USA.
[Li, Tingwen] Natl Energy Technol Lab, 3610 Collins Ferry Rd, Morgantown, WV 26507 USA.
[Li, Tingwen] AECOM, 3610 Collins Ferry Rd, Morgantown, WV 26507 USA.
RP Sarkar, A (reprint author), Pacific Northwest Natl Lab, Fundamental & Computat Sci Directorate, POB 999,MSIN K7-90, Richland, WA 99352 USA.; Sarkar, A (reprint author), Pfizer Inc, Worldwide Res & Dev, MS 8156-014,Eastern Point Rd, Groton, CT 06340 USA.
EM aviksarkar2@gmail.com
FU U.S. Department of Energy, Office of Fossil Energy's Carbon Capture
Simulation Initiative (CCSI) through the National Energy Technology
Laboratory; U.S. Department of Energy [DE-AC05-76RL01830]
FX This work, performed at the Pacific Northwest National Laboratory, was
funded by the U.S. Department of Energy, Office of Fossil Energy's
Carbon Capture Simulation Initiative (CCSI) through the National Energy
Technology Laboratory. Pacific Northwest National Laboratory is operated
by Battelle Memorial Institute for the U.S. Department of Energy under
Contract no. DE-AC05-76RL01830. We also express our gratitude to
Christian C. Milioli (currently at Princeton University), Jean-Francois
Dietiker (NETL), and Janine Carney (NETL) for their assistance with this
work.
NR 33
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U1 6
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PU PERGAMON-ELSEVIER SCIENCE LTD
PI OXFORD
PA THE BOULEVARD, LANGFORD LANE, KIDLINGTON, OXFORD OX5 1GB, ENGLAND
SN 0009-2509
EI 1873-4405
J9 CHEM ENG SCI
JI Chem. Eng. Sci.
PD OCT 2
PY 2016
VL 152
BP 443
EP 456
DI 10.1016/j.ces.2016.06.023
PG 14
WC Engineering, Chemical
SC Engineering
GA DT5SG
UT WOS:000381542300040
ER
PT J
AU Provino, A
Sangeetha, NS
Dhar, SK
Smetana, V
Gschneidner, KA
Pecharsky, VK
Manfrinetti, P
Mudring, AV
AF Provino, Alessia
Sangeetha, Nediadath S.
Dhar, Sudesh K.
Smetana, Volodymyr
Gschneidner, Karl A., Jr.
Pecharsky, Vitalij K.
Manfrinetti, Pietro
Mudring, Anja-Verena
TI New R3Pd5 Compounds (R = Sc, Y, Gd-Lu): Formation and Stability, Crystal
Structure, and Antiferromagnetism
SO CRYSTAL GROWTH & DESIGN
LA English
DT Article
ID PHASE-DIAGRAM; PD SYSTEM; PALLADIUM SYSTEM; THERMODYNAMIC ASSESSMENT;
PHYSICAL-PROPERTIES; ALLOYING BEHAVIOR; INDIUM SYSTEM; RARE-EARTHS;
EQUILIBRIA; YTTERBIUM
AB The phases reported in the literature as "R2Pd3" (R = rare earth element) have been reinvestigated. The exact stoichiometric composition of this series of compounds, which form for R = Sc, Y, and from Gd to Lu, including Yb, was found to be R3Pd5. All of them crystallize in the orthorhombic Pu3Pd5 structure type (oS32-Cmcm). The crystal structure has been refined from both single crystal (for Tb3Pd5) and powder X-ray diffraction data (for Tb3Pd5, Ho3Pd5, and Tm3Pd5). These ccmpounds represent the first example of a binary phase formed by R and Pd adopting the Pu3Pd5-type featuring two crystallographic nonequivalent sites for the R atoms in the unit cell (the Wyckoff sites 4c and 8e). The variation of the lattice parameters and unit cell volume along the series strictly-follows the trend of the lanthanide contraction. An extrapolation of the volume contraction versus the R3+ ionic radius gives an atomic volume: of 29.74 angstrom(3) for Yb in the hypothetical trivalent metallic state (under normal conditions). The formation temperatures and mechanisms, peritectic reaction, and stability ranges have also been investigated. It turns out that Gd3Pd5 is a high temperature phase; it was not possible to quench this compound as a metastable phase, at room temperature, to be measured. In the light Of our results, most of the R-Pd phase diagrams need to be revised. The magnetization, heat capacity,, and electrical resistivity have been Measured for Tb3Pd5, Dy3Pd5, Ho3Pd5, and Er3Pd5. They order antiferromagnetically at low temperatures, each undergoing two transitions, T-N1 and T-N2 (with T-N1, going from 13.5 to 5.1 K and T-N2 going from 6.5 to 3.6 K, respectively for Tb and Ho compounds). From our data we cannot distinguish: whether the two rare earth sublattices sequentially order magnetically at T-N1 and T-N2, respectively, or whether they are simultaneously involved in both transitions. The electronic structure calculations predict antiferromagnetic ordering also for Gd3Pd5. Y(3)Ed(5) is a Pauli paramagnet.
C1 [Provino, Alessia; Manfrinetti, Pietro] Univ Genoa, Dept Chem, I-16146 Genoa, Italy.
[Provino, Alessia; Smetana, Volodymyr; Gschneidner, Karl A., Jr.; Pecharsky, Vitalij K.; Manfrinetti, Pietro; Mudring, Anja-Verena] Iowa State Univ, Ames Lab, USDOE, Ames, IA 50011 USA.
[Provino, Alessia; Manfrinetti, Pietro] Inst SPIN CNR, I-16152 Genoa, Italy.
[Sangeetha, Nediadath S.; Dhar, Sudesh K.] Tata Inst Fundamental Res, Dept Condensed Matter Phys & Mat Sci, Bombay 400005, Maharashtra, India.
[Smetana, Volodymyr; Gschneidner, Karl A., Jr.; Pecharsky, Vitalij K.; Mudring, Anja-Verena] Iowa State Univ, Dept Mat Sci & Engn, Ames, IA 50011 USA.
[Sangeetha, Nediadath S.] Iowa State Univ, Ames Lab, Ames, IA 50011 USA.
RP Provino, A (reprint author), Univ Genoa, Dept Chem, I-16146 Genoa, Italy.; Provino, A (reprint author), Iowa State Univ, Ames Lab, USDOE, Ames, IA 50011 USA.; Provino, A (reprint author), Inst SPIN CNR, I-16152 Genoa, Italy.
EM alessia.provino@spin.cnr.it
FU University of Genova; Office of the Basic Energy Sciences; DOE
[DE-AC02-07CH11358]
FX A.P. would like to thank the University of Genova for supporting the
research leave in 2015. The research was partly supported by the Office
of the Basic Energy Sciences. Materials Sciences and Engineering
Division of the USDOE Ames Laboratory is operated for DOE by Iowa State
University under Contract DE-AC02-07CH11358.
NR 66
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U1 0
U2 0
PU AMER CHEMICAL SOC
PI WASHINGTON
PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA
SN 1528-7483
EI 1528-7505
J9 CRYST GROWTH DES
JI Cryst. Growth Des.
PD OCT
PY 2016
VL 16
IS 10
BP 6001
EP 6015
DI 10.1021/acs.cgd.6b01045
PG 15
WC Chemistry, Multidisciplinary; Crystallography; Materials Science,
Multidisciplinary
SC Chemistry; Crystallography; Materials Science
GA DY2WI
UT WOS:000384952400048
ER
PT J
AU Gamarnik, D
Misra, S
AF Gamarnik, David
Misra, Sidhant
TI A Note on Alternating Minimization Algorithm for the Matrix Completion
Problem
SO IEEE SIGNAL PROCESSING LETTERS
LA English
DT Article
DE Alternating minimization; compressive sensing; low-rank matrix
completion
ID ENTRIES
AB We consider the problem of reconstructing a low-rank matrix from a subset of its entries and analyze two variants of the so-called alternating minimization algorithm, which has been proposed in the past. We establish thatwhen the underlying matrix has rank one, has positive bounded entries, and the graph underlying the revealed entries has diameter which is logarithmic in the size of the matrix, both algorithms succeed in reconstructing the matrix approximately in polynomial time starting from an arbitrary initialization. We further provide simulation results which suggest that the second variant which is based on the message passing type updates performs significantly better.
C1 [Gamarnik, David] MIT, Ctr Operat Res, Cambridge, MA 02139 USA.
[Gamarnik, David] MIT, Sloan Sch Management, 77 Massachusetts Ave, Cambridge, MA 02139 USA.
[Misra, Sidhant] Los Alamos Natl Lab, Ctr Non Linear Studies, Los Alamos, NM 87545 USA.
RP Gamarnik, D (reprint author), MIT, Ctr Operat Res, Cambridge, MA 02139 USA.; Gamarnik, D (reprint author), MIT, Sloan Sch Management, 77 Massachusetts Ave, Cambridge, MA 02139 USA.
EM gamarnik@mit.edu; sidhant@lanl.gov
FU National Science Foundation of China [CMMI-1335155]
FX This work was supported by the National Science Foundation of China
under Grant CMMI-1335155.
NR 9
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Z9 0
U1 1
U2 1
PU IEEE-INST ELECTRICAL ELECTRONICS ENGINEERS INC
PI PISCATAWAY
PA 445 HOES LANE, PISCATAWAY, NJ 08855-4141 USA
SN 1070-9908
EI 1558-2361
J9 IEEE SIGNAL PROC LET
JI IEEE Signal Process. Lett.
PD OCT
PY 2016
VL 23
IS 10
BP 1340
EP 1343
DI 10.1109/LSP.2016.2576979
PG 4
WC Engineering, Electrical & Electronic
SC Engineering
GA EM0NB
UT WOS:000395013900001
ER
PT J
AU Kleban, M
Senatore, L
AF Kleban, Matthew
Senatore, Leonardo
TI Inhomogeneous anisotropic cosmology
SO JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS
LA English
DT Article
DE gravity; initial conditions and eternal universe; cosmological
simulations; inflation
ID INFLATIONARY UNIVERSE; RELATIVITY; CURVATURE; FLATNESS; HORIZON
AB In homogeneous and isotropic Friedmann-Robertson-Walker cosmology, the topology of the universe determines its ultimate fate. If the Weak Energy Condition is satisfied, open and flat universes must expand forever, while closed cosmologies can recollapse to a Big Crunch. A similar statement holds for homogeneous but anisotropic (Bianchi) universes. Here, we prove that arbitrarily inhomogeneous and anisotropic cosmologies with "flat" (including toroidal) and "open" (including compact hyperbolic) spatial topology that are initially expanding must continue to expand forever at least in some region at a rate bounded from below by a positive number, despite the presence of arbitrarily large density fluctuations and/or the formation of black holes. Because the set of 3-manifold topologies is countable, a single integer determines the ultimate fate of the universe, and, in a specific sense, most 3-manifolds are "flat" or "open". Our result has important implications for inflation: if there is a positive cosmological constant (or suitable inflationary potential) and initial conditions for the inflaton, cosmologies with "flat" or "open" topology must expand forever in some region at least as fast as de Sitter space, and are therefore very likely to begin inflationary expansion eventually, regardless of the scale of the inflationary energy or the spectrum and amplitude of initial inhomogeneities and gravitational waves. Our result is also significant for numerical general relativity, which often makes use of periodic (toroidal) boundary conditions.
C1 [Kleban, Matthew] NYU, Ctr Cosmol & Particle Phys, 4 Washington Pl, New York, NY 10003 USA.
[Senatore, Leonardo] Stanford Univ, Stanford Inst Theoret Phys, 382 Via Pueblo Mall, Stanford, CA 94306 USA.
[Senatore, Leonardo] Stanford Univ, Dept Phys, 382 Via Pueblo Mall, Stanford, CA 94306 USA.
[Senatore, Leonardo] Stanford Univ, Kavli Inst Particle Astrophys & Cosmol, 2575 Sand Hill Rd,M-S 29, Menlo Pk, CA 94025 USA.
[Senatore, Leonardo] SLAC, 2575 Sand Hill Rd,M-S 29, Menlo Pk, CA 94025 USA.
RP Kleban, M (reprint author), NYU, Ctr Cosmol & Particle Phys, 4 Washington Pl, New York, NY 10003 USA.
EM kleban@nyu.edu; senatore@stanford.edu
FU NSF [PHY-1214302]; DOE [DE-FG02-12ER41854]
FX The work of MK is supported in part by the NSF through grant
PHY-1214302, and he acknowledges membership at the NYU-ECNU Joint
Physics Research Institute in Shanghai. LS is supported by DOE Early
Career Award DE-FG02-12ER41854. We would like to thank John Barrow, Jeff
Cheeger, Paolo Creminelli, Atish Dabholkar, Will East, Eli Grigsby,
Andrei Gruzinov, Andrei Linde, Nemanja Kaloper, Bruce Kleiner, Alberto
Nicolis, Massimo Porrati, Neil Turok, Alex Vilenkin, Giovanni Villadoro,
Bob Wald, and Matias Zaldarriaga for very useful conversations.
NR 22
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Z9 0
U1 0
U2 0
PU IOP PUBLISHING LTD
PI BRISTOL
PA TEMPLE CIRCUS, TEMPLE WAY, BRISTOL BS1 6BE, ENGLAND
SN 1475-7516
J9 J COSMOL ASTROPART P
JI J. Cosmol. Astropart. Phys.
PD OCT
PY 2016
IS 10
AR 022
DI 10.1088/1475-7516/2016/10/022
PG 12
WC Astronomy & Astrophysics; Physics, Particles & Fields
SC Astronomy & Astrophysics; Physics
GA EL4FZ
UT WOS:000394578400027
ER
PT J
AU Muckley, ES
Miller, N
Jacobs, CB
Gredig, T
Ivanov, IN
AF Muckley, Eric S.
Miller, Nicholas
Jacobs, Christopher B.
Gredig, Thomas
Ivanov, Ilia N.
TI Morphology-defined interaction of copper phthalocyanine with O-2/H2O
SO JOURNAL OF PHOTONICS FOR ENERGY
LA English
DT Article
DE copper phthalocyanine; morphology; oxygen; water; quartz crystal
microbalance; adsorption
ID FIELD-EFFECT TRANSISTOR; THIN-FILM; GAS SENSOR; OXYGEN; TEMPERATURE;
SUBSTRATE; THICKNESS; WATER
AB Copper phthalocyanine (CuPc) is an important hole transport layer for organic photo-voltaics (OPVs), but interaction with ambient gas/vapor may lead to changes in its electronic properties and limit OPV device lifetimes. CuPc films of thickness 25 and 100 nm were grown by thermal sublimation at 25 degrees C,150 degrees C, and 250 degrees C in order to vary morphology. We measured electrical resistance and film mass in situ during exposure to controlled pulses of O-2 and H2O vapor. CuPc films deposited at 250 degrees C showed a factor of 5 higher uptake of O-2 as detected by a quartz crystal microbalance (QCM), possibly due to the formation of beta-CuPc at T > 200 degrees C which allows higher O-2 mobility between stacked molecules. While weight-based measurements stabilize after similar to 10 min of gas exposure, resistance response stabilizes over times >1 h, suggesting that mass change occurs by rapid adsorption at active surface sites whereas resistive response is dominated by slow diffusion of adsorbates into the bulk film. The 25 nm films exhibit higher resistive response than 100 nm films after an hour of O-2/H2O exposure due to fast analyte diffusion down to the film/electrode interface. We found evidence of decoupling of CuPc from the gold-coated QCM crystal due to preferential adsorption of O-2/H2O molecules on gold. (C) 2016 Society of Photo-Optical Instrumentation Engineers (SPIE)
C1 [Muckley, Eric S.; Jacobs, Christopher B.; Ivanov, Ilia N.] Oak Ridge Natl Lab, Ctr Nanophase Mat Sci, POB 2008, Oak Ridge, TN 37831 USA.
[Muckley, Eric S.] Univ Tennessee, Bredesen Ctr Energy Sci & Engn, 444 Greve Hall,821 Volunteer Blvd, Knoxville, TN 37996 USA.
[Miller, Nicholas; Gredig, Thomas] Calif State Univ Long Beach, Dept Phys & Astron, 1250 Bellflower Blvd, Long Beach, CA 90840 USA.
RP Muckley, ES (reprint author), Oak Ridge Natl Lab, Ctr Nanophase Mat Sci, POB 2008, Oak Ridge, TN 37831 USA.; Muckley, ES (reprint author), Univ Tennessee, Bredesen Ctr Energy Sci & Engn, 444 Greve Hall,821 Volunteer Blvd, Knoxville, TN 37996 USA.
EM muckleyes@ornl.gov; ivanovin@ornl.gov
NR 34
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U1 0
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PU SPIE-SOC PHOTO-OPTICAL INSTRUMENTATION ENGINEERS
PI BELLINGHAM
PA 1000 20TH ST, PO BOX 10, BELLINGHAM, WA 98225 USA
SN 1947-7988
J9 J PHOTON ENERGY
JI J. Photonics Energy
PD OCT-DEC
PY 2016
VL 6
IS 4
AR 045501
DI 10.1117/1.JPE.6.045501
PG 9
WC Materials Science, Multidisciplinary; Optics; Physics, Applied
SC Materials Science; Optics; Physics
GA EM8BL
UT WOS:000395536100014
ER
PT J
AU Daftari, IK
Mishra, KK
Singh, RP
Shadoan, DJ
Phillips, TL
AF Daftari, I. K.
Mishra, K. K.
Singh, R. P.
Shadoan, D. J.
Phillips, T. L.
TI Design and Evolution of the Control System for Ocular Proton Beam
Therapy
SO INTERNATIONAL JOURNAL OF RADIATION ONCOLOGY BIOLOGY PHYSICS
LA English
DT Meeting Abstract
CT 58th Annual Meeting of the American-Society-for-Radiation-Oncology
(ASTRO)
CY SEP 25-28, 2016
CL Boston, MA
SP Amer Soc Radiat Oncol
C1 [Daftari, I. K.; Mishra, K. K.; Singh, R. P.; Shadoan, D. J.; Phillips, T. L.] Univ Calif San Francisco, San Francisco, CA 94143 USA.
[Singh, R. P.; Shadoan, D. J.] Lawrence Berkeley Natl Lab, Berkeley, CA USA.
[Phillips, T. L.] Univ Arizona, Tucson, AZ USA.
NR 0
TC 0
Z9 0
U1 0
U2 0
PU ELSEVIER SCIENCE INC
PI NEW YORK
PA 360 PARK AVE SOUTH, NEW YORK, NY 10010-1710 USA
SN 0360-3016
EI 1879-355X
J9 INT J RADIAT ONCOL
JI Int. J. Radiat. Oncol. Biol. Phys.
PD OCT 1
PY 2016
VL 96
IS 2
SU S
MA 3701
BP E694
EP E694
PG 1
WC Oncology; Radiology, Nuclear Medicine & Medical Imaging
SC Oncology; Radiology, Nuclear Medicine & Medical Imaging
GA EB8QL
UT WOS:000387655804280
ER
PT J
AU Henke, LE
Olsen, JR
Green, OL
Yang, D
Zhao, T
Olsen, LA
Wooten, H
Li, H
Rodriguez, VL
McClain, B
Curcuru, A
Robinson, CG
Bradley, JD
Michalski, JM
Mutic, S
Parikh, PJ
Kashani, R
AF Henke, L. E.
Olsen, J. R.
Green, O. L.
Yang, D.
Zhao, T.
Olsen, L. A.
Wooten, H.
Li, H.
Rodriguez, V. L.
McClain, B.
Curcuru, A.
Robinson, C. G.
Bradley, J. D.
Michalski, J. M.
Mutic, S.
Parikh, P. J.
Kashani, R.
TI Online Adaptive Magnetic Resonancee-Guided (OAMR)-Stereotactic Body
Radiation Therapy for Abdominal Malignancies: Prospective Dosimetric
Results from a Phase 1 Trial
SO INTERNATIONAL JOURNAL OF RADIATION ONCOLOGY BIOLOGY PHYSICS
LA English
DT Meeting Abstract
CT 58th Annual Meeting of the American-Society-for-Radiation-Oncology
(ASTRO)
CY SEP 25-28, 2016
CL Boston, MA
SP Amer Soc Radiat Oncol
C1 [Henke, L. E.; Curcuru, A.; Bradley, J. D.; Kashani, R.] Washington Univ, Sch Med, Dept Radiat Oncol, St Louis, MO USA.
[Olsen, J. R.] Univ Colorado Denver, Sch Med, Denver, CO USA.
[Green, O. L.; Yang, D.; Li, H.; Rodriguez, V. L.; McClain, B.; Michalski, J. M.; Mutic, S.; Parikh, P. J.] Washington Univ, Sch Med, St Louis, MO USA.
[Zhao, T.; Robinson, C. G.] Washington Univ, Dept Radiat Oncol, St Louis, MO USA.
[Olsen, L. A.] Mem Hosp UCHlth, Colorado Springs, CO USA.
[Wooten, H.] Los Alamos Natl Lab, Los Alamos, NM USA.
NR 0
TC 0
Z9 0
U1 0
U2 0
PU ELSEVIER SCIENCE INC
PI NEW YORK
PA 360 PARK AVE SOUTH, NEW YORK, NY 10010-1710 USA
SN 0360-3016
EI 1879-355X
J9 INT J RADIAT ONCOL
JI Int. J. Radiat. Oncol. Biol. Phys.
PD OCT 1
PY 2016
VL 96
IS 2
SU S
MA 1139
BP S222
EP S223
PG 2
WC Oncology; Radiology, Nuclear Medicine & Medical Imaging
SC Oncology; Radiology, Nuclear Medicine & Medical Imaging
GA EB8QL
UT WOS:000387655805142
ER
PT J
AU Strassert, JFH
Mikaelyan, A
Woyke, T
Brune, A
AF Strassert, Juergen F. H.
Mikaelyan, Aram
Woyke, Tanja
Brune, Andreas
TI Genome analysis of 'Candidatus Ancillula trichonymphae', first
representative of a deep-branching clade of Bifidobacteriales,
strengthens evidence for convergent evolution in flagellate
endosymbionts
SO ENVIRONMENTAL MICROBIOLOGY REPORTS
LA English
DT Article
ID TERMITE-GUT; HOST PROTIST; SYMBIONTS; ENDOMICROBIA; BACTERIA;
LIGNOCELLULOSE; MICROBIOTA; FIXATION; NITROGEN; PHYLUM
AB The flagellate protists in the hindgut of lower termites play an essential role in the digestion of lignocellulose. Most flagellate species are associated with host-specific symbionts from various bacterial lineages, which typically lack cultured representatives. In this study, we analyzed the genome of 'Candidatus Ancillula trichonymphae', an endosymbiont of Trichonympha flagellates from dry-wood termites, which represents a novel, family-level lineage of uncultured Actinobacteria encountered so far only in termite guts. The draft genome of 'Ca. A. trichonymphae' (ca. 1.48 Mbp; 95% complete) revealed a purely fermentative metabolism that is probably fueled by xylose, N-acetyl-glucosamine and glycerol 3-phosphate acquired from the flagellate host. The absence of fructose bisphosphate aldolase and the presence of a complete gene set encoding the phosphoketolase pathway underscore the sister position of the new lineage to Bifidobacteriaceae. The preservation of the pathways for the assimilation of ammonia and the synthesis of 18 amino acids and several cofactors and vitamins suggests that 'Ca. A. trichonymphae' -like other endosymbionts of termite gut flagellates-provides essential amino acids and vitamins to its host. Our findings corroborate the emerging concept that numerous lineages of unrelated flagellate endosymbionts have convergently evolved to fill similar ecological niches.
C1 [Strassert, Juergen F. H.; Mikaelyan, Aram; Brune, Andreas] Max Planck Inst Terr Microbiol, Dept Biogeochem, Marburg, Germany.
[Woyke, Tanja] US DOE, Joint Genome Inst, Walnut Creek, CA USA.
[Strassert, Juergen F. H.] Univ British Columbia, Dept Bot, Vancouver, BC, Canada.
RP Brune, A (reprint author), Max Planck Inst Terr Microbiol, Dept Biogeochem, Marburg, Germany.
EM brune@mpi-marburg.mpg.de
FU Max Planck Society; U.S. Department of Energy Joint Genome Institute
FX This research was funded by the Max Planck Society. Genome sequencing
was supported by the U.S. Department of Energy Joint Genome Institute.
We thank Dr. Rudiger Plarre (Federal Institute for Materials Research
and Testing, Berlin) for providing termites and Dr. Geert Michel and his
group (Charite, Campus Benjamin Franklin, Berlin) for assistance with
the use of their micromanipulation/laser dissection system.
NR 33
TC 1
Z9 1
U1 0
U2 0
PU WILEY-BLACKWELL
PI HOBOKEN
PA 111 RIVER ST, HOBOKEN 07030-5774, NJ USA
SN 1758-2229
J9 ENV MICROBIOL REP
JI Environ. Microbiol. Rep.
PD OCT
PY 2016
VL 8
IS 5
SI SI
BP 865
EP 873
DI 10.1111/1758-2229.12451
PG 9
WC Environmental Sciences; Microbiology
SC Environmental Sciences & Ecology; Microbiology
GA EM0IP
UT WOS:000395002300041
ER
PT J
AU Ade, PAR
Aghanim, N
Akrami, Y
Aluri, PK
Arnaud, M
Ashdown, M
Aumont, J
Baccigalupi, C
Banday, AJ
Barreiro, RB
Bartolo, N
Basak, S
Battaner, E
Benabed, K
Benoit, A
Benoit-Levy, A
Bernard, JP
Bersanelli, M
Bielewicz, P
Bock, JJ
Bonaldi, A
Bonavera, L
Bond, JR
Borrill, J
Bouchet, FR
Boulanger, F
Bucher, M
Burigana, C
Butler, RC
Calabrese, E
Cardoso, JF
Casaponsa, B
Catalano, A
Challinor, A
Chamballu, A
Chiang, HC
Christensen, PR
Church, S
Clements, DL
Colombi, S
Colombo, LPL
Combet, C
Contreras, D
Couchot, F
Coulais, A
Crill, BP
Cruz, M
Curto, A
Cuttaia, F
Danese, L
Davies, RD
Davis, RJ
de Bernardis, P
de Rosa, A
de Zotti, G
Delabrouille, J
Desert, FX
Diego, JM
Dole, H
Donzelli, S
Dore, O
Douspis, M
Ducout, A
Dupac, X
Efstathiou, G
Elsner, F
Ensslin, TA
Eriksen, HK
Fantaye, Y
Ferguson, J
Fernandez-Cobos, R
Finelli, F
Forni, O
Frailis, M
Fraisse, AA
Franceschi, E
Frejsel, A
Frolov, A
Galeotta, S
Galli, S
Ganga, K
Gauthier, C
Ghosh, T
Giard, M
Giraud-Heraud, Y
Gjerlow, E
Gonzalez-Nuevo, J
Gorski, KM
Gratton, S
Gregorio, A
Gruppuso, A
Gudmundsson, JE
Hansen, FK
Hanson, D
Harrison, DL
Henrot-Versille, S
Hernandez-Monteagudo, C
Herranz, D
Hildebrandt, SR
Hivon, E
Hobson, M
Holmes, WA
Hornstrup, A
Hovest, W
Huang, Z
Huffenberger, KM
Hurier, G
Jaffe, AH
Jaffe, TR
Jones, WC
Juvela, M
Keihanen, E
Keskitalo, R
Kim, J
Kisner, TS
Knoche, J
Kunz, M
Kurki-Suonio, H
Lagache, G
Lahteenmaki, A
Lamarre, JM
Lasenby, A
Lattanzi, M
Lawrence, CR
Leonardi, R
Lesgourgues, J
Levrier, F
Liguori, M
Lilje, PB
Linden-Vornle, M
Liu, H
Lopez-Caniego, M
Lubin, PM
Macias-Perez, JF
Maggio, G
Maino, D
Mandolesi, N
Mangilli, A
Marinucci, D
Maris, M
Martin, PG
Martinez-Gonzalez, E
Masi, S
Matarrese, S
McGehee, P
Meinhold, PR
Melchiorri, A
Mendes, L
Mennella, A
Migliaccio, M
Mikkelsen, K
Mitra, S
Miville-Deschenes, MA
Molinari, D
Moneti, A
Montier, L
Morgante, G
Mortlock, D
Moss, A
Munshi, D
Murphy, JA
Naselsky, P
Nati, F
Natoli, P
Netterfield, CB
Norgaard-Nielsen, HU
Noviello, F
Novikov, D
Novikov, I
Oxborrow, CA
Paci, F
Pagano, L
Pajot, F
Pant, N
Paoletti, D
Pasian, F
Patanchon, G
Pearson, TJ
Perdereau, O
Perotto, L
Perrotta, F
Pettorino, V
Piacentini, F
Piat, M
Pierpaoli, E
Pietrobon, D
Plaszczynski, S
Pointecouteau, E
Polenta, G
Popa, L
Pratt, GW
Prezeau, G
Prunet, S
Puget, JL
Rachen, JP
Rebolo, R
Reinecke, M
Remazeilles, M
Renault, C
Renzi, A
Ristorcelli, I
Rocha, G
Rosset, C
Rossetti, M
Rotti, A
Roudier, G
Rubino-Martin, JA
Rusholme, B
Sandri, M
Santos, D
Savelainen, M
Savini, G
Scott, D
Seiffert, MD
Shellard, EPS
Souradeep, T
Spencer, LD
Stolyarov, V
Stompor, R
Sudiwala, R
Sunyaev, R
Sutton, D
Suur-Uski, AS
Sygnet, JF
Tauber, JA
Terenzi, L
Toffolatti, L
Tomasi, M
Tristram, M
Trombetti, T
Tucci, M
Tuovinen, J
Valenziano, L
Valiviita, J
Van Tent, B
Vielva, P
Villa, F
Wade, LA
Wandelt, BD
Wehus, IK
Yvon, D
Zacchei, A
Zibin, JP
Zonca, A
AF Ade, P. A. R.
Aghanim, N.
Akrami, Y.
Aluri, P. K.
Arnaud, M.
Ashdown, M.
Aumont, J.
Baccigalupi, C.
Banday, A. J.
Barreiro, R. B.
Bartolo, N.
Basak, S.
Battaner, E.
Benabed, K.
Benoit, A.
Benoit-Levy, A.
Bernard, J. -P
Bersanelli, M.
Bielewicz, P.
Bock, J. J.
Bonaldi, A.
Bonavera, L.
Bond, J. R.
Borrill, J.
Bouchet, F. R.
Boulanger, F.
Bucher, M.
Burigana, C.
Butler, R. C.
Calabrese, E.
Cardoso, J. -F.
Casaponsa, B.
Catalano, A.
Challinor, A.
Chamballu, A.
Chiang, H. C.
Christensen, P. R.
Church, S.
Clements, D. L.
Colombi, S.
Colombo, L. P. L.
Combet, C.
Contreras, D.
Couchot, F.
Coulais, A.
Crill, B. P.
Cruz, M.
Curto, A.
Cuttaia, F.
Danese, L.
Davies, R. D.
Davis, R. J.
de Bernardis, P.
de Rosa, A.
de Zotti, G.
Delabrouille, J.
Desert, F. -X.
Diego, J. M.
Dole, H.
Donzelli, S.
Dore, O.
Douspis, M.
Ducout, A.
Dupac, X.
Efstathiou, G.
Elsner, F.
Ensslin, T. A.
Eriksen, H. K.
Fantaye, Y.
Ferguson, J.
Fernandez-Cobos, R.
Finelli, F.
Forni, O.
Frailis, M.
Fraisse, A. A.
Franceschi, E.
Frejsel, A.
Frolov, A.
Galeotta, S.
Galli, S.
Ganga, K.
Gauthier, C.
Ghosh, T.
Giard, M.
Giraud-Heraud, Y.
Gjerlow, E.
Gonzalez-Nuevo, J.
Gorski, K. M.
Gratton, S.
Gregorio, A.
Gruppuso, A.
Gudmundsson, J. E.
Hansen, F. K.
Hanson, D.
Harrison, D. L.
Henrot-Versille, S.
Hernandez-Monteagudo, C.
Herranz, D.
Hildebrandt, S. R.
Hivon, E.
Hobson, M.
Holmes, W. A.
Hornstrup, A.
Hovest, W.
Huang, Z.
Huffenberger, K. M.
Hurier, G.
Jaffe, A. H.
Jaffe, T. R.
Jones, W. C.
Juvela, M.
Keihanen, E.
Keskitalo, R.
Kim, J.
Kisner, T. S.
Knoche, J.
Kunz, M.
Kurki-Suonio, H.
Lagache, G.
Lahteenmaki, A.
Lamarre, J. -M.
Lasenby, A.
Lattanzi, M.
Lawrence, C. R.
Leonardi, R.
Lesgourgues, J.
Levrier, F.
Liguori, M.
Lilje, P. B.
Linden-Vornle, M.
Liu, H.
Lopez-Caniego, M.
Lubin, P. M.
Macias-Perez, J. F.
Maggio, G.
Maino, D.
Mandolesi, N.
Mangilli, A.
Marinucci, D.
Maris, M.
Martin, P. G.
Martinez-Gonzalez, E.
Masi, S.
Matarrese, S.
McGehee, P.
Meinhold, P. R.
Melchiorri, A.
Mendes, L.
Mennella, A.
Migliaccio, M.
Mikkelsen, K.
Mitra, S.
Miville-Deschenes, M. -A.
Molinari, D.
Moneti, A.
Montier, L.
Morgante, G.
Mortlock, D.
Moss, A.
Munshi, D.
Murphy, J. A.
Naselsky, P.
Nati, F.
Natoli, P.
Netterfield, C. B.
Norgaard-Nielsen, H. U.
Noviello, F.
Novikov, D.
Novikov, I.
Oxborrow, C. A.
Paci, F.
Pagano, L.
Pajot, F.
Pant, N.
Paoletti, D.
Pasian, F.
Patanchon, G.
Pearson, T. J.
Perdereau, O.
Perotto, L.
Perrotta, F.
Pettorino, V.
Piacentini, F.
Piat, M.
Pierpaoli, E.
Pietrobon, D.
Plaszczynski, S.
Pointecouteau, E.
Polenta, G.
Popa, L.
Pratt, G. W.
Prezeau, G.
Prunet, S.
Puget, J. -L.
Rachen, J. P.
Rebolo, R.
Reinecke, M.
Remazeilles, M.
Renault, C.
Renzi, A.
Ristorcelli, I.
Rocha, G.
Rosset, C.
Rossetti, M.
Rotti, A.
Roudier, G.
Rubino-Martin, J. A.
Rusholme, B.
Sandri, M.
Santos, D.
Savelainen, M.
Savini, G.
Scott, D.
Seiffert, M. D.
Shellard, E. P. S.
Souradeep, T.
Spencer, L. D.
Stolyarov, V.
Stompor, R.
Sudiwala, R.
Sunyaev, R.
Sutton, D.
Suur-Uski, A. -S.
Sygnet, J. -F.
Tauber, J. A.
Terenzi, L.
Toffolatti, L.
Tomasi, M.
Tristram, M.
Trombetti, T.
Tucci, M.
Tuovinen, J.
Valenziano, L.
Valiviita, J.
Van Tent, B.
Vielva, P.
Villa, F.
Wade, L. A.
Wandelt, B. D.
Wehus, I. K.
Yvon, D.
Zacchei, A.
Zibin, J. P.
Zonca, A.
CA Planck Collaboration
TI Planck 2015 results XVI. Isotropy and statistics of the CMB
SO ASTRONOMY & ASTROPHYSICS
LA English
DT Article
DE cosmology: observations; cosmic background radiation; polarization;
methods: data analysis; methods: statistical
ID MICROWAVE-ANISOTROPY-PROBE; OBSERVATIONS COSMOLOGICAL INTERPRETATION;
PRIMORDIAL NON-GAUSSIANITY; 5-YEAR WMAP DATA; COLD SPOT; BACKGROUND
ANISOTROPY; SKY MAPS; MINKOWSKI FUNCTIONALS; SPHERICAL WAVELETS; POWER
ASYMMETRY
AB We test the statistical isotropy and Gaussianity of the cosmic microwave background (CMB) anisotropies using observations made by the Planck satellite. Our results are based mainly on the full Planck mission for temperature, but also include some polarization measurements. In particular, we consider the CMB anisotropy maps derived from the multi-frequency Planck data by several component-separation methods. For the temperature anisotropies, we find excellent agreement between results based on these sky maps over both a wry large fraction of the sky and a broad range of angular scales, establishing that potential foreground residuals do not affect our studies. Tests of skewness, kurtosis, multi-normality, N-point functions, and Minkowski functionals indicate consistency with Gaussianity, while a power deficit at large angular scales is manifested in several ways, for example low map variance. The results of a peak statistics analysis are consistent with the expectations of a Gaussian random field. The "Cold Spot" is detected with several methods, including map kurtosis, peak statistics, and mean temperature profile. We thoroughly probe the large-scale dipolar power asymmetry, detecting it with several independent tests, and address the subject of a posteriori correction. Tests of directionality suggest the presence of angular clustering from large to small scales, but at a significance that is dependent on the details of the approach. We perform the first examination of polarization data, finding the morphology of stacked peaks to be consistent with the expectations of statistically isotropic simulations. Where they overlap, these results are consistent with the Planck 2013 analysis based on the nominal mission data and provide our most thorough view of the statistics of the CMB fluctuations to date.
C1 [Bucher, M.; Cardoso, J. -F.; Delabrouille, J.; Ganga, K.; Gauthier, C.; Giraud-Heraud, Y.; Patanchon, G.; Piat, M.; Remazeilles, M.; Rosset, C.; Roudier, G.; Stompor, R.] Univ Paris Diderot, CNRS IN2P3, CEA Irfu, APC,AstroParticule & Cosmol,Observ Paris,Sorbonne, 10 Rue Alice Domon & Leonie Duquet, F-75205 Paris 13, France.
[Lahteenmaki, A.] Aalto Univ, Metsahovi Radio Observ, POB 13000, Aalto 00076, Finland.
[Lahteenmaki, A.] Dept Radio Sci & Engn, POB 13000, Aalto 00076, Finland.
[Kunz, M.] African Inst Math Sci, 6-8 Melrose Rd, Cape Town, South Africa.
[Natoli, P.; Polenta, G.] Agenzia Spaziale Italiana Sci Data Ctr, Via Politecn Snc, I-00133 Rome, Italy.
[Lagache, G.] Aix Marseille Univ, CNRS, LAM, UMR 7326, F-13388 Marseille, France.
[Ashdown, M.; Curto, A.; Hobson, M.; Lasenby, A.; Stolyarov, V.] Univ Cambridge, Cavendish Lab, Astrophys Grp, JJ Thomson Ave, Cambridge CB3 0HE, England.
[Chiang, H. C.] Univ KwaZulu Natal, Sch Math Stat & Comp Sci, Astrophys & Cosmol Res Unit, Westville Campus,Private Bag X54001, ZA-4000 Durban, South Africa.
[Bond, J. R.; Hanson, D.; Huang, Z.; Martin, P. G.; Miville-Deschenes, M. -A.] Univ Toronto, CITA, 60 St George St, Toronto, ON M5S 3H8, Canada.
[Banday, A. J.; Bernard, J. -P; Bielewicz, P.; Forni, O.; Giard, M.; Jaffe, T. R.; Montier, L.; Pointecouteau, E.] CNRS, IRAP, 9 Av Colonel Roche,BP 44346, F-31028 Toulouse 4, France.
[Tuovinen, J.] Trinity Coll Dublin, CRANN, Dublin, Ireland.
[Bock, J. J.; Crill, B. P.; Dore, O.; Hildebrandt, S. R.; Pearson, T. J.; Prezeau, G.; Rocha, G.; Seiffert, M. D.] CALTECH, Pasadena, CA 91125 USA.
[Challinor, A.; Ferguson, J.; Shellard, E. P. S.] Univ Cambridge, Ctr Theoret Cosmol, DAMTP, Wilberforce Rd, Cambridge CB3 0WA, England.
[Hernandez-Monteagudo, C.] CEFCA, Plaza San Juan 1,Planta 2, Teruel 44001, Spain.
[Borrill, J.; Keskitalo, R.] Lawrence Berkeley Natl Lab, Computat Cosmol Ctr, Berkeley, CA USA.
[Rebolo, R.] CSIC, Madrid, Spain.
[Chamballu, A.; Yvon, D.] CEA Saclay, DSM Irfu SPP, F-91191 Gif Sur Yvette, France.
[Hornstrup, A.; Linden-Vornle, M.; Norgaard-Nielsen, H. U.; Oxborrow, C. A.] Tech Univ Denmark, Natl Space Inst, DTU Space, Elektrovej 327, DK-2800 Lyngby, Denmark.
[Kunz, M.; Tucci, M.] Univ Geneva, Dept Phys Theor, 24 Quai E Ansermet, CH-1211 Geneva, Switzerland.
[Rebolo, R.; Rubino-Martin, J. A.] Univ La Laguna, Dept Astrofis, San Cristobal la Laguna 38206, Tenerife, Spain.
[Gonzalez-Nuevo, J.; Toffolatti, L.] Univ Oviedo, Dept Fis, Avda Calvo Sotelo S-N, Oviedo 33003, Spain.
[Cruz, M.] Univ Cantabria, Dept Matemat Estadist & Computac, Avda Castros S-N, E-39005 Santander, Spain.
[Netterfield, C. B.] Univ Toronto, Dept Astron & Astrophys, 50 St George St, Toronto, ON, Canada.
[Rachen, J. P.] Radboud Univ Nijmegen, IMAPP, Dept Astrophys, POB 9010, NL-6500 GL Nijmegen, Netherlands.
[Contreras, D.; Scott, D.; Zibin, J. P.] Univ British Columbia, Dept Phys & Astron, 6224 Agr Rd, Vancouver, BC, Canada.
[Colombo, L. P. L.; Pierpaoli, E.] Univ Southern Calif, Dana & David Dornsife Coll Letter Arts & Sci, Dept Phys & Astron, Los Angeles, CA 90089 USA.
[Elsner, F.] UCL, Dept Phys & Astron, London WC1E 6BT, England.
[Huffenberger, K. M.] Florida State Univ, Dept Phys, Keen Phys Bldg,77 Chieftan Way, Tallahassee, FL 32306 USA.
[Juvela, M.; Keihanen, E.; Kurki-Suonio, H.; Savelainen, M.; Suur-Uski, A. -S.; Valiviita, J.] Univ Helsinki, Dept Phys, Gustaf Hallstromin Katu 2a, Helsinki 00100, Finland.
[Chiang, H. C.; Fraisse, A. A.; Gudmundsson, J. E.; Jones, W. C.; Nati, F.] Princeton Univ, Dept Phys, Princeton, NJ 08544 USA.
[Lubin, P. M.; Meinhold, P. R.; Zonca, A.] Univ Calif Santa Barbara, Dept Phys, Santa Barbara, CA 93106 USA.
[Wandelt, B. D.] Univ Illinois, Dept Phys, 1110 West Green St, Urbana, IL USA.
[Bartolo, N.; Liguori, M.; Matarrese, S.] Univ Padua, Dipartimento Fis & Astron G Galilei, Via Marzolo 8, I-35131 Padua, Italy.
[Burigana, C.; Lattanzi, M.; Mandolesi, N.; Natoli, P.] Univ Ferrara, Dipartimento Fis & Sci Terra, Via Saragat 1, I-44122 Ferrara, Italy.
[de Bernardis, P.; Masi, S.; Melchiorri, A.; Pagano, L.; Piacentini, F.] Univ Roma La Sapienza, Dipartimento Fis, Ple A Moro 2, Rome, Italy.
[Bersanelli, M.; Maino, D.; Mennella, A.; Rossetti, M.; Tomasi, M.] Univ Milan, Dipartimento Fis, Via Celoria 16, Milan, Italy.
[Benoit-Levy, A.; Gregorio, A.] Univ Trieste, Dipartimento Fis, Via A Valerio 2, Trieste, Italy.
[Fantaye, Y.; Marinucci, D.; Renzi, A.] Univ Roma Tor Vergata, Dipartimento Matemat, Via Ric Sci 1, Rome, Italy.
[Christensen, P. R.; Liu, H.; Naselsky, P.] Niels Bohr Inst, Discovery Ctr, 17 Blegdamsvej, Copenhagen, Denmark.
[Dupac, X.; Leonardi, R.; Lopez-Caniego, M.; Mendes, L.] European Space Agcy, ESAC, Planck Sci Off, Camino Bajo Castillo S-N, Madrid 28692, Spain.
[Tauber, J. A.] European Space Agcy, Estec, Keplerlaan 1, NL-2201 AZ Noordwijk, Netherlands.
[Terenzi, L.] Univ E Campus, Fac Ingn, Via Isimbardi 10, I-22060 Novedrate, CO, Italy.
[Matarrese, S.] Ist Nazl Fis Nucl, Gran Sasso Sci Inst, Viale F Crispi 7, I-67100 Laquila, Italy.
[Pettorino, V.] HGSFP, Philosophenweg 16, D-69120 Heidelberg, Germany.
[Pettorino, V.] Heidelberg Univ, Dept Theoret Phys, Philosophenweg 16, D-69120 Heidelberg, Germany.
[Kurki-Suonio, H.; Lahteenmaki, A.; Savelainen, M.; Suur-Uski, A. -S.; Valiviita, J.] Univ Helsinki, Helsinki Inst Phys, Gustaf Hallstromin Katu 2, Helsinki, Finland.
[de Zotti, G.] Osserv Astron Padova, INAF, Vicolo Osservatorio 5, Padua, Italy.
[Polenta, G.] Osserv Astron Roma, INAF, Via Frascati 33, Monte Porzio Catone, Italy.
[Frailis, M.; Galeotta, S.; Gregorio, A.; Maggio, G.; Maris, M.; Pasian, F.; Zacchei, A.] Osserv Astron Trieste, INAF, Via GB Tiepolo 11, Trieste, Italy.
[Burigana, C.; Butler, R. C.; Cuttaia, F.; de Rosa, A.; Finelli, F.; Franceschi, E.; Gruppuso, A.; Mandolesi, N.; Molinari, D.; Morgante, G.; Natoli, P.; Paoletti, D.; Sandri, M.; Terenzi, L.; Toffolatti, L.; Trombetti, T.; Valenziano, L.; Villa, F.] IASF Bologna, INAF, Via Gobetti 101, Bologna, Italy.
[Bersanelli, M.; Donzelli, S.; Maino, D.; Mennella, A.; Rossetti, M.; Tomasi, M.] IASF Milano, INAF, Via E Bassini 15, Milan, Italy.
[Burigana, C.; Finelli, F.; Paoletti, D.] Ist Nazl Fis Nucl, Sez Bologna, Via Irnerio 46, I-40126 Bologna, Italy.
[Melchiorri, A.; Pagano, L.] Univ Roma Sapienza, Ist Nazl Fis Nucl, Sez Roma 1, Piazzale Aldo Moro 2, I-00185 Rome, Italy.
[Renzi, A.] Univ Roma Tor Vergata, Ist Nazl Fis Nucl, Sez Roma 2, Via Ric Sci 1, Rome, Italy.
[Gregorio, A.] Ist Nazl Fis Nucl, Natl Inst Nucl Phys, Via Valerio 2, I-34127 Trieste, Italy.
[Desert, F. -X.] Univ Grenoble Alpes, IPAG, CNRS, F-38000 Grenoble, France.
[Aluri, P. K.; Mitra, S.; Pant, N.; Rotti, A.; Souradeep, T.] Pune Univ Campus, Post Bag 4, Pune 411007, Maharashtra, India.
[Clements, D. L.; Ducout, A.; Jaffe, A. H.; Mortlock, D.] Imperial Coll London, Blackett Lab, Astrophys Grp, Prince Consort Rd, London SW7 2AZ, England.
[McGehee, P.; Pearson, T. J.; Rusholme, B.] CALTECH, Infrared Proc & Anal Ctr, Pasadena, CA 91125 USA.
[Benoit, A.] Univ Grenoble 1, CNRS, Inst Neel, 25 Rue Martyrs, Grenoble, France.
[Dole, H.] Inst Univ France, 103 Bd St Michel, F-75005 Paris, France.
[Aghanim, N.; Aumont, J.; Boulanger, F.; Chamballu, A.; Dole, H.; Douspis, M.; Ghosh, T.; Hurier, G.; Kunz, M.; Lagache, G.; Mangilli, A.; Miville-Deschenes, M. -A.; Pajot, F.; Puget, J. -L.; Remazeilles, M.] Univ Paris 11, CNRS, Inst Astrophys Spatiale, UMR 8617, Batiment 121, F-91440 Orsay, France.
[Benabed, K.; Benoit-Levy, A.; Bouchet, F. R.; Cardoso, J. -F.; Colombi, S.; Ducout, A.; Elsner, F.; Hivon, E.; Moneti, A.; Prunet, S.; Sygnet, J. -F.; Wandelt, B. D.] CNRS, Inst Astrophys Paris, UMR 7095, 98 Bis Blvd Arago, F-75014 Paris, France.
[Lesgourgues, J.] Rhein Westfal TH Aachen, Inst Theoret Teilchenphys & Kosmol, D-52056 Aachen, Germany.
[Popa, L.] Inst Space Sci, Bucharest 077125, Romania.
[Challinor, A.; Efstathiou, G.; Gratton, S.; Harrison, D. L.; Migliaccio, M.; Sutton, D.] Univ Cambridge, Inst Astron, Madingley Rd, Cambridge CB3 0HA, England.
[Akrami, Y.; Eriksen, H. K.; Gjerlow, E.; Hansen, F. K.; Lilje, P. B.; Mikkelsen, K.] Univ Oslo, Inst Theoret Astrophys, N-0371 Oslo, Norway.
[Rebolo, R.; Rubino-Martin, J. A.] Inst Astrofis Canarias, C Via Lactea S-N, San Cristobal la Laguna 38205, Tenerife, Spain.
[Barreiro, R. B.; Bonavera, L.; Casaponsa, B.; Curto, A.; Diego, J. M.; Fernandez-Cobos, R.; Gonzalez-Nuevo, J.; Herranz, D.; Lopez-Caniego, M.; Martinez-Gonzalez, E.; Molinari, D.; Toffolatti, L.; Vielva, P.] Univ Cantabria, CSIC, Inst Fis Cantabria, Avda Castros S-N, Santander 39005, Spain.
[Bartolo, N.; Liguori, M.; Matarrese, S.] Ist Nazl Fis Nucl, Sez Padova, Via Marzolo 8, I-35131 Padua, Italy.
[Bock, J. J.; Colombo, L. P. L.; Crill, B. P.; Dore, O.; Gorski, K. M.; Hanson, D.; Hildebrandt, S. R.; Holmes, W. A.; Lawrence, C. R.; Mitra, S.; Pietrobon, D.; Prezeau, G.; Rocha, G.; Roudier, G.; Seiffert, M. D.; Wade, L. A.; Wehus, I. K.] CALTECH, Jet Prop Lab, 4800 Oak Grove Dr, Pasadena, CA 91125 USA.
[Bonaldi, A.; Davies, R. D.; Davis, R. J.; Noviello, F.; Remazeilles, M.] Univ Manchester, Jodrell Bank Ctr Astrophys, Sch Phys & Astron, Alan Turing Bldg,Oxford Rd, Manchester M13 9PL, Lancs, England.
[Galli, S.] Univ Chicago, Kavli Inst Cosmol Phys, Chicago, IL 60637 USA.
[Ashdown, M.; Challinor, A.; Curto, A.; Gratton, S.; Harrison, D. L.; Lasenby, A.; Migliaccio, M.; Sutton, D.] Univ Cambridge, Kavli Inst Cosmol Cambridge, Cambridge CB3 0HA, England.
[Stolyarov, V.] Kazan Fed Univ, 18 Kremlyovskaya St, Kazan 420008, Russia.
[Couchot, F.; Henrot-Versille, S.; Mangilli, A.; Perdereau, O.; Plaszczynski, S.; Tristram, M.] Univ Paris 11, CNRS, IN2P3, LAL, Orsay, France.
[Catalano, A.; Coulais, A.; Lamarre, J. -M.; Levrier, F.; Roudier, G.] CNRS, Observ Paris, LERMA, 61 Ave Observ, F-75014 Paris, France.
[Arnaud, M.; Chamballu, A.; Pratt, G. W.] Univ Paris Diderot, CEA Saclay, CEA DSM CNRS, IRFU,Serv Astrophys,Lab AIM, Bat 709, F-91191 Gif Sur Yvette, France.
[Cardoso, J. -F.] CNRS, Lab Traitement & Commun Informat, UMR 5141, 46 Rue Barrault, F-75634 Paris 13, France.
[Cardoso, J. -F.] Telecom ParisTech, 46 Rue Barrault, F-75634 Paris 13, France.
[Catalano, A.; Combet, C.; Macias-Perez, J. F.; Perotto, L.; Renault, C.; Santos, D.] Univ Grenoble Alpes, CNRS, IN2P3, Lab Phys Subatom & Cosmol, 53 Rue Martyrs, F-38026 Grenoble, France.
[Van Tent, B.] Univ Paris 11, Lab Phys Theor, Batiment 210, F-91405 Orsay, France.
[Van Tent, B.] CNRS, Batiment 210, F-91405 Orsay, France.
[Kisner, T. S.] Lawrence Berkeley Natl Lab, Berkeley, CA USA.
[Novikov, D.; Novikov, I.] Russian Acad Sci, Ctr Astro Space, Lebedev Phys Inst, 84-32 Profsoyuznaya St, Moscow 117997, Russia.
[Gauthier, C.] Natl Taiwan Univ, Leung Ctr Cosmol & Particle Astrophys, Taipei 10617, Taiwan.
[Ensslin, T. A.; Hernandez-Monteagudo, C.; Hovest, W.; Kim, J.; Knoche, J.; Rachen, J. P.; Reinecke, M.; Sunyaev, R.] Max Planck Inst Astrophys, Karl Schwarzschild Str 1, D-85741 Garching, Germany.
[Hanson, D.] McGill Univ, McGill Phys, Ernest Rutherford Phys Bldg,3600 Rue Univ, Montreal, PQ H3A 2T8, Canada.
[Murphy, J. A.] Natl Univ Ireland, Dept Expt Phys, Maynooth, Kildare, Ireland.
[Bielewicz, P.] Nicolaus Copernicus Astron Ctr, Bartycka 18, PL-00716 Warsaw, Poland.
[Christensen, P. R.; Frejsel, A.; Liu, H.; Naselsky, P.; Novikov, I.] Niels Bohr Inst, Blegdamsvej 17, DK-2100 Copenhagen, Denmark.
[Savini, G.] UCL, Opt Sci Lab, Gower St, London, England.
[Baccigalupi, C.; Basak, S.; Bielewicz, P.; Danese, L.; de Zotti, G.; Paci, F.; Perrotta, F.] SISSA, Astrophys Sect, Via Bonomea 265, I-34136 Trieste, Italy.
[Ade, P. A. R.; Munshi, D.; Spencer, L. D.; Sudiwala, R.] Cardiff Univ, Sch Phys & Astron, Queens Buildings, Cardiff CF24 3AA, S Glam, Wales.
[Moss, A.] Univ Nottingham, Sch Phys & Astron, Nottingham NG7 2RD, England.
[Frolov, A.] Simon Fraser Univ, Dept Phys, 8888 Univ Dr, Burnaby, BC, Canada.
[Bouchet, F. R.] UPMC, Sorbonne Univ, Inst Astrophys Paris, UMR 7095, 98 Bis Blvd Arago, F-75014 Paris, France.
[Sunyaev, R.] Russian Acad Sci, Space Res Inst IKI, Profsoyuznaya Str 84-32, Moscow 117997, Russia.
[Borrill, J.] Univ Calif Berkeley, Space Sci Lab, Berkeley, CA 94720 USA.
[Stolyarov, V.] Russian Acad Sci, Special Astrophys Observ, Nizhnii Arkhyz 369167, Zelenchukskiy R, Russia.
[Church, S.] Stanford Univ, Dept Phys, Varian Phys Bldg,382 Via Pueblo Mall, Stanford, CA 94305 USA.
[Calabrese, E.] Univ Oxford, Subdept Astrophys, Keble Rd, Oxford OX1 3RH, England.
[Lesgourgues, J.] CERN, PH TH, Div Theory, CH-1211 Geneva 23, Switzerland.
[Benabed, K.; Benoit-Levy, A.; Colombi, S.; Elsner, F.; Hivon, E.; Prunet, S.; Wandelt, B. D.] Univ Paris 06, UMR 7095, 98 Bis Blvd Arago, F-75014 Paris, France.
[Banday, A. J.; Bernard, J. -P; Forni, O.; Giard, M.; Jaffe, T. R.; Montier, L.; Pointecouteau, E.; Ristorcelli, I.] Univ Toulouse, UPS OMP, IRAP, F-31028 Toulouse 4, France.
[Battaner, E.] Univ Granada, Fac Ciencias, Dept Fis Teor & Cosmos, E-18071 Granada, Spain.
[Battaner, E.] Univ Granada, Inst Carlos Fis Teor & Computac 1, E-18071 Granada, Spain.
[Akrami, Y.] Heidelberg Univ, Inst Theoret Phys, Philosophenweg 16, D-69120 Heidelberg, Germany.
[Gorski, K. M.] Univ Warsaw Observ, Aleje Ujazdowskie 4, PL-00478 Warsaw, Poland.
RP Banday, AJ (reprint author), CNRS, IRAP, 9 Av Colonel Roche,BP 44346, F-31028 Toulouse 4, France.; Banday, AJ (reprint author), Univ Toulouse, UPS OMP, IRAP, F-31028 Toulouse 4, France.
EM anthony.banday@irap.omp.eu
RI Lahteenmaki, Anne/L-5987-2013; Barreiro, Rita Belen/N-5442-2014;
bonavera, laura/E-9368-2017; Gonzalez-Nuevo, Joaquin/I-3562-2014;
Herranz, Diego/K-9143-2014; Colombo, Loris/J-2415-2016;
OI Juvela, Mika/0000-0002-5809-4834; Molinari, Diego/0000-0002-7799-3915;
Zacchei, Andrea/0000-0003-0396-1192; Toffolatti,
Luigi/0000-0003-2645-7386; Lilje, Per/0000-0003-4324-7794; Liu,
Hao/0000-0003-4410-5827; Paoletti, Daniela/0000-0003-4761-6147; Nati,
Federico/0000-0002-8307-5088; Savini, Giorgio/0000-0003-4449-9416;
Pierpaoli, Elena/0000-0002-7957-8993; Huang, Zhiqi/0000-0002-1506-1063;
Kurki-Suonio, Hannu/0000-0002-4618-3063; Barreiro, Rita
Belen/0000-0002-6139-4272; bonavera, laura/0000-0001-8039-3876;
Gonzalez-Nuevo, Joaquin/0000-0003-1354-6822; Herranz,
Diego/0000-0003-4540-1417; Colombo, Loris/0000-0003-4572-7732;
Stolyarov, Vladislav/0000-0001-8151-828X; Valiviita,
Jussi/0000-0001-6225-3693; Hurier, Guillaume/0000-0002-1215-0706
FU ESA; CNES (France); CNRS/INSU-IN2P3-INP (France); ASI (Italy); CNR
(Italy); INAF (Italy); NASA (USA); DoE (USA); STFC (UK); UKSA (UK); CSIC
(Spain); MINECO (Spain); JA (Spain); RES (Spain); Tekes (Finland); AoF
(Finland); CSC (Finland); DLR (Germany); MPG (Germany); CSA (Canada);
DTU Space (Denmark); SER/SSO (Switzerland); RCN (Norway); SFI (Ireland);
FCT/MCTES (Portugal); ERC; PRACE (EU)
FX The Planck Collaboration acknowledges the support of: ESA; CNES and
CNRS/INSU-IN2P3-INP (France); ASI, CNR, and INAF (Italy); NASA and DoE
(USA); STFC and UKSA (UK); CSIC, MINECO, JA, and RES (Spain); Tekes,
AoF, and CSC (Finland); DLR and MPG (Germany); CSA (Canada); DTU Space
(Denmark); SER/SSO (Switzerland); RCN (Norway); SFI (Ireland); FCT/MCTES
(Portugal); ERC and PRACE (EU). A description of the Planck
Collaboration and a list of its members, indicating which technical or
scientific activities they have been involved in, can be found at
http://www.cosmos.esaint/web/planck/planch-collaboration. Some of the
results in this paper have been derived using the HEALPix package.
NR 157
TC 1
Z9 1
U1 0
U2 0
PU EDP SCIENCES S A
PI LES ULIS CEDEX A
PA 17, AVE DU HOGGAR, PA COURTABOEUF, BP 112, F-91944 LES ULIS CEDEX A,
FRANCE
SN 1432-0746
J9 ASTRON ASTROPHYS
JI Astron. Astrophys.
PD OCT
PY 2016
VL 594
AR Al6
DI 10.1051/0004-6361/201526681
PG 62
WC Astronomy & Astrophysics
SC Astronomy & Astrophysics
GA DZ4MG
UT WOS:000385832200023
ER
PT J
AU Grecu, M
Olson, WS
Munchak, SJ
Ringerud, S
Liao, L
Haddad, Z
Kelley, BL
McLaughlin, SF
AF Grecu, Mircea
Olson, William S.
Munchak, Stephen Joseph
Ringerud, Sarah
Liao, Liang
Haddad, Ziad
Kelley, Bartie L.
McLaughlin, Steven F.
TI The GPM Combined Algorithm
SO JOURNAL OF ATMOSPHERIC AND OCEANIC TECHNOLOGY
LA English
DT Article
ID RAIN-PROFILING ALGORITHM; TRMM PRECIPITATION RADAR; MICROWAVE RADIATIVE
PROPERTIES; DROP SIZE DISTRIBUTION; PART II; MULTIPLE-SCATTERING;
MELTING-LAYER; RADIOMETER; FREQUENCIES; RETRIEVALS
AB In this paper, the operational Global Precipitation Measurement (GPM) mission combined radar-radiometer algorithm is thoroughly described. The operational combined algorithm is designed to reduce uncertainties in GPM Core Observatory precipitation estimates by effectively integrating complementary information from the GPM Dual-Frequency Precipitation Radar (DPR) and the GPM Microwave Imager (GMI) into an optimal, physically consistent precipitation product. Although similar in many respects to previously developed combined algorithms, the GPM combined algorithm has several unique features that are specifically designed to meet the GPM objectives of deriving, based on GPM Core Observatory information, accurate and physically consistent precipitation estimates from multiple spaceborne instruments, and ancillary environmental data from reanalyses. The algorithm features an optimal estimation framework based on a statistical formulation of the Gauss-Newton method, a parameterization for the nonuniform distribution of precipitation within the radar fields of view, a methodology to detect and account for multiple scattering in Ka-band DPR observations, and a statistical deconvolution technique that allows for an efficient sequential incorporation of radiometer information into DPR precipitation retrievals.
C1 [Grecu, Mircea; Liao, Liang] Morgan State Univ, Goddard Earth Sci Technol & Res, Baltimore, MD 21239 USA.
[Grecu, Mircea] NASA GSFC, Atmospheres Lab, Greenbelt, MD USA.
[Olson, William S.] Univ Maryland, Joint Ctr Earth Syst Technol, Baltimore, MD 21201 USA.
[Olson, William S.; Munchak, Stephen Joseph; Ringerud, Sarah; Liao, Liang] NASA GSFC, Mesoscale Atmospher Proc Lab, 8800 Greenbelt Rd,MC 612, Greenbelt, MD 20771 USA.
[Ringerud, Sarah] Oak Ridge Associated Univ, Oak Ridge, TN USA.
[Haddad, Ziad] CALTECH, Jet Prop Lab, Pasadena, CA USA.
[Kelley, Bartie L.; McLaughlin, Steven F.] Sci Syst & Applicat Inc, Lanham, MD USA.
RP Grecu, M (reprint author), NASA GSFC, Mesoscale Atmospher Proc Lab, 8800 Greenbelt Rd,MC 612, Greenbelt, MD 20771 USA.
EM mircea.grecu-1@nasa.gov
FU NASA PMM project [NNX13AF85G]
FX This work was supported by the NASA PMM project (NNX13AF85G). The
authors thank Drs. Ramesh Kakar (NASA headquarters) and Gail
Skofronick-Jackson (GPM project scientist) for their support of this
effort. The authors would also like to thank the PMM combined algorithm
team members, Benjamin Johnson, Lin Tian, Kwo-Sen Kuo, and Hirohiko
Masunaga, for their contributions to the overall algorithm development
effort. In addition, the authors are grateful to Lawrence Woltz and NASA
Precipitation Processing System personnel for their operational support,
David Bolvin for his help with GPCP data, and Drs. Pierre Kirstetter and
Chris Kidd for their insights into the use of MRMS and other ground
validation products. The authors also thank Dr. Robin Hogan for making
public the source code of the fast multiple-scattering model, and three
anonymous reviewers for their comments and suggestions.
NR 57
TC 0
Z9 0
U1 2
U2 2
PU AMER METEOROLOGICAL SOC
PI BOSTON
PA 45 BEACON ST, BOSTON, MA 02108-3693 USA
SN 0739-0572
EI 1520-0426
J9 J ATMOS OCEAN TECH
JI J. Atmos. Ocean. Technol.
PD OCT
PY 2016
VL 33
IS 10
BP 2225
EP 2245
DI 10.1175/JTECH-D-16-0019.1
PG 21
WC Engineering, Ocean; Meteorology & Atmospheric Sciences
SC Engineering; Meteorology & Atmospheric Sciences
GA EL3RG
UT WOS:000394536000005
ER
PT J
AU Wu, ZP
Gao, WZ
Wang, X
Kang, M
Hwang, M
Kang, YC
Gevogian, V
Muljadi, E
AF Wu, Ziping
Gao, Wenzhong
Wang, Xiao
Kang, Moses
Hwang, Min
Kang, Yong Cheol
Gevogian, Vahan
Muljadi, Eduard
TI Improved inertial control for permanent magnet synchronous generator
wind turbine generators
SO IET RENEWABLE POWER GENERATION
LA English
DT Article
ID FREQUENCY-CONTROL; POWER-SYSTEMS
AB With increasing integrations of large-scale systems based on permanent magnet synchronous generator wind turbine generators (PMSG-WTGs), the overall inertial response of a power system will tend to deteriorate as a result of the decoupling of rotor speed and grid frequency through the power converter as well as the scheduled retirement of conventional synchronous generators. Thus, PMSG-WTGs can provide value to an electric grid by contributing to the system's inertial response through the inherent kinetic energy stored in their rotating masses and fast power converter control. In this study, an improved inertial control method based on the maximum power point tracking operation curve is introduced to enhance the overall frequency support capability of PMSG-WTGs in the case of large supply-demand imbalances. Moreover, this method is implemented in the CART2-PMSG integrated model in MATLAB/Simulink to investigate its impact on the wind turbine's structural loads during the inertial response process. Simulation results indicate that the proposed method can effectively reduce the frequency nadir, arrest the rate of change of frequency, and alleviate the secondary frequency dip while imposing no negative impact on the major mechanical components of the wind turbine.
C1 [Wu, Ziping; Gao, Wenzhong; Wang, Xiao] Univ Denver, Dept Elect & Comp Engn, Denver, CO 80208 USA.
[Kang, Moses; Hwang, Min; Kang, Yong Cheol] Chonbuk Natl Univ, Dept Elect Engn, Jeonju 561756, South Korea.
[Gevogian, Vahan; Muljadi, Eduard] Natl Renewable Energy Lab, Power Syst Engn Ctr, Golden, CO USA.
RP Gao, WZ (reprint author), Univ Denver, Dept Elect & Comp Engn, Denver, CO 80208 USA.
EM wenzhong.gao@du.edu
FU U.S. Department of Energy [DE-AC36-08-GO28308]; NREL
FX Authors' contribution to this work was supported by the U.S. Department
of Energy under contract no. DE-AC36-08-GO28308 with the NREL. This work
is collaboration among the NREL. The authors acknowledge the support
provided by Paul Fleming and Andrew Scholbrock of NREL during the
preparation of this paper and the future implementation of this method
on the CART turbine.
NR 25
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Z9 0
U1 2
U2 2
PU INST ENGINEERING TECHNOLOGY-IET
PI HERTFORD
PA MICHAEL FARADAY HOUSE SIX HILLS WAY STEVENAGE, HERTFORD SG1 2AY, ENGLAND
SN 1752-1416
EI 1752-1424
J9 IET RENEW POWER GEN
JI IET Renew. Power Gener.
PD OCT
PY 2016
VL 10
IS 9
BP 1366
EP 1373
DI 10.1049/iet-rpg.2016.0125
PG 8
WC GREEN & SUSTAINABLE SCIENCE & TECHNOLOGY; Energy & Fuels; Engineering,
Electrical & Electronic
SC Science & Technology - Other Topics; Energy & Fuels; Engineering
GA EL3KH
UT WOS:000394517500013
ER
PT J
AU Provino, A
Steinberg, S
Smetana, V
Pararmanik, U
Manfrinetti, P
Dhar, SK
Mudring, AV
AF Provino, Alessia
Steinberg, Simon
Smetana, Volodymyr
Pararmanik, Uday
Manfrinetti, Pietro
Dhar, Sudesh K.
Mudring, Anja-Verena
TI Gold in the Layered Structures of R3Au7Sn3: From Relativity to
Versatility
SO CRYSTAL GROWTH & DESIGN
LA English
DT Article
ID AU-GA SYSTEM; ICOSAHEDRAL QUASI-CRYSTAL; RARE-EARTH-METALS;
INTERMETALLIC COMPOUNDS; ZR3AL2-TYPE STRUCTURE; NEUTRON-DIFFRACTION;
PHASES; TRANSITION; STANNIDES; INDIUM
AB A series of isotypes of ternary rare earth element-gold-tetrel intermetallic compounds have been synthesized, and their structures and properties have been characterized. R3Au7Sn3 (R = Y, La-Nd, Sm, Gd-Tm, Lu) crystallize with the hexagonal Gd3Au7Sn3 prototype (Pearson symbol hP26; P6(3)/m, a = 8.110-8.372 angstrom, c = 9.351-9.609 angstrom, V-cell = 532.7-583.3 angstrom(3), Z = 2), an ordered variant of the Cu10Sn3-type. Their structures are built up by GdPt2Sn-type layers, which feature edge-sharing Sn@Au-6 trigonal antiprisms connected by trigonal R-3 groups. Additional insertion of gold atoms leads to the formation of new homoatomic Au clusters, Au@Au-6; alternatively, the structure can be considered as a superstructural polyhedral packing of the ZrBeSi-type. The magnetization, heat capacity, and electrical resistivity have been measured for R3Au7Sn3 (R = Ce, Pr, Nd, and Tb). All four compounds order antiferromagnetically with the highest T-N of 13 K for Tb3Au7Sn3. In Ce3Au7Sn3, which has a T-N of 2.9 K, the heat capacity and electrical resistivity data in zero and applied fields indicate the presence of Kondo interaction. The coefficient of the linear term in the electronic heat capacity, gamma, derived from the heat capacity data below 0.5 K is 211 mJ/Ce mol K-2, suggesting strong electronic correlations due to the Kondo interaction. The electronic structure calculations based on the projector augmented wave method for particular representatives of the series suggest different tendencies of the localized R-4f atomic orbitals (AOs) to hybridize with the valence states. LMTO-based bonding analysis on the nonmagnetic La3Au7Sn3 indicates that the integrated crystal orbital Hamilton populations are dominated by the heteroatomic Au-Sn contacts; however, contributions from La-Au and La-Sn separations are significant, both together exceeding 40% in the overall bonding. Homoatomic Au-Au interactions are evident for the Au@Au-6 units, but, despite of the high atomic concentration of Au in the compound, they do not dominate the entire bonding picture.
C1 [Provino, Alessia; Steinberg, Simon; Smetana, Volodymyr; Manfrinetti, Pietro; Mudring, Anja-Verena] Iowa State Univ, Ames Lab, US DOE, Ames, IA 50011 USA.
[Provino, Alessia; Manfrinetti, Pietro] Univ Genoa, Dept Chem, Via Dodecaneso 31, I-16146 Genoa, Italy.
[Provino, Alessia; Manfrinetti, Pietro] Inst SPIN CNR, Corso Perrone 24, I-16152 Genoa, Italy.
[Steinberg, Simon; Smetana, Volodymyr; Mudring, Anja-Verena] Iowa State Univ, Dept Mat Sci & Engn, Ames, IA 50011 USA.
[Dhar, Sudesh K.] TIFR, Dept Condensed Matter Phys & Mat Sci, Homi Bhabha Rd, Bombay 400005, Maharashtra, India.
[Pararmanik, Uday] Indian Inst Technol, Dept Phys, Kanpur 208016, Uttar Pradesh, India.
RP Mudring, AV (reprint author), Iowa State Univ, Ames Lab, US DOE, Ames, IA 50011 USA.; Mudring, AV (reprint author), Iowa State Univ, Dept Mat Sci & Engn, Ames, IA 50011 USA.
EM mudring@iastate.edu
RI Smetana, Volodymyr/C-1340-2015
FU Office of the Basic Energy Sciences, Materials Sciences Division, U.S.
DOE; DOE [DE-AC02-07CH11358]
FX The research was supported by the Office of the Basic Energy Sciences,
Materials Sciences Division, U.S. DOE. Ames Laboratory is operated for
DOE by Iowa State University under Contract DE-AC02-07CH11358.
NR 83
TC 0
Z9 0
U1 1
U2 1
PU AMER CHEMICAL SOC
PI WASHINGTON
PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA
SN 1528-7483
EI 1528-7505
J9 CRYST GROWTH DES
JI Cryst. Growth Des.
PD OCT
PY 2016
VL 16
IS 10
BP 5657
EP 5668
DI 10.1021/acs.cgd.6b00478
PG 12
WC Chemistry, Multidisciplinary; Crystallography; Materials Science,
Multidisciplinary
SC Chemistry; Crystallography; Materials Science
GA DY2WI
UT WOS:000384952400012
ER
PT J
AU Kim, JS
Chen, J
Garcia, HE
AF Kim, Jong Suk
Chen, Jun
Garcia, Humberto E.
TI Modeling, control, and dynamic performance analysis of a reverse osmosis
desalination plant integrated within hybrid energy systems
SO ENERGY
LA English
DT Article
DE Desalination; Reverse osmosis; Variable renewable generation; Hybrid
energy systems; Flexible load resource; Ancillary service
ID SPIRAL WOUND MODULES; SEAWATER DESALINATION; MEMBRANE REJECTION;
FOSSIL-FUEL; RO SYSTEMS; ELECTRICITY; SIMULATION; NUCLEAR; WATER;
OPTIMIZATION
AB An RO (reverse osmosis) desalination plant is proposed as an effective, FLR (flexible load resource) to be integrated into HES (hybrid energy systems) to support various types of ancillary services to the electric grid, under variable operating conditions. To study the dynamic analysis of such system, special attention is given here to the detailed dynamic modeling and control design of RO desalination process that employs a spiral-wound membrane module. In particular, the solution-diffusion model modified with the concentration polarization theory is applied to predict RO performance over a large range of operating conditions. Simulation results involving several case studies suggest that an RO desalination plant can provide operational flexibility to participate in energy management at the utility scale by dynamically optimizing the use of excess electrical energy. The incorporation of additional commodity (fresh water) produced from a FLR allows a broader range of HES operations for maximizing overall system performance and profitability. Published by Elsevier Ltd.
C1 [Kim, Jong Suk; Chen, Jun; Garcia, Humberto E.] Idaho Natl Lab, 750 Univ Blvd, Idaho Falls, ID 83415 USA.
RP Kim, JS (reprint author), Idaho Natl Lab, 750 Univ Blvd, Idaho Falls, ID 83415 USA.
EM jkim0916@gmail.com
RI Kim, Jong Suk/B-9660-2017;
OI Kim, Jong Suk/0000-0001-6179-4420; Chen, Jun/0000-0002-0934-8519
FU Energy Security Initiative under the U.S. Department of Energy
[DE-AC07-05ID14517]; N-R HES (Nuclear-Renewable Hybrid Energy Systems)
Program at INL (Idaho National Laboratory) under the U.S. Department of
Energy [DE-AC07-05ID14517]
FX This research is supported by the Energy Security Initiative and the N-R
HES (Nuclear-Renewable Hybrid Energy Systems) Program at INL (Idaho
National Laboratory) under the U.S. Department of Energy contract
DE-AC07-05ID14517. The authors would like to acknowledge the leadership
of Drs. Shannon M. Bragg-Sitton and Richard D. Boardman in the (N-R HES)
Program at INL, whose contributions made this work possible.
NR 54
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Z9 6
U1 0
U2 0
PU PERGAMON-ELSEVIER SCIENCE LTD
PI OXFORD
PA THE BOULEVARD, LANGFORD LANE, KIDLINGTON, OXFORD OX5 1GB, ENGLAND
SN 0360-5442
EI 1873-6785
J9 ENERGY
JI Energy
PD OCT 1
PY 2016
VL 112
BP 52
EP 66
DI 10.1016/j.energy.2016.05.050
PG 15
WC Thermodynamics; Energy & Fuels
SC Thermodynamics; Energy & Fuels
GA DY7OL
UT WOS:000385318700006
ER
PT J
AU Gutierrez, C
Kim, CJ
Brown, L
Schiros, T
Nordlund, D
Lochocki, EB
Shen, KM
Park, J
Pasupathy, AN
AF Gutierrez, Christopher
Kim, Cheol-Joo
Brown, Lola
Schiros, Theanne
Nordlund, Dennis
Lochocki, Edward B.
Shen, Kyle M.
Park, Jiwoong
Pasupathy, Abhay N.
TI Imaging chiral symmetry breaking from Kekule bond order in graphene
SO NATURE PHYSICS
LA English
DT Article
ID METAL-METAL INTERFACES; EPITAXIAL GRAPHENE; RELAXATION; SOLITONS;
SURFACE
AB Chirality-or 'handedness'-is a symmetry property crucial to fields as diverse as biology, chemistry and high-energy physics. In graphene, chiral symmetry emerges naturally as a consequence of the carbon honeycomb lattice. This symmetry can be broken by interactions that couple electrons with opposite momenta in graphene. Here we directly visualize the formation of Kekule bond order, one such phase of broken chiral symmetry, in an ultraflat graphene sheet grown epitaxially on a copper substrate. We show that its origin lies in the interactions between individual vacancies in the copper substrate that are mediated electronically by the graphene. We show that this interaction causes the bonds in graphene to distort, creating a phase with broken chiral symmetry. The Kekule ordering is robust at ambient temperature and atmospheric conditions, indicating that intercalated atoms may be harnessed to drive graphene and other two-dimensional materials towards electronically desirable and exotic collective phases.
C1 [Gutierrez, Christopher; Pasupathy, Abhay N.] Columbia Univ, Dept Phys, 538 W 120th St, New York, NY 10027 USA.
[Kim, Cheol-Joo; Brown, Lola; Park, Jiwoong] Cornell Univ, Dept Chem & Chem Biol, Ithaca, NY 14853 USA.
[Schiros, Theanne] SUNY Fashion Inst Technol, Dept Sci & Math, New York, NY 10001 USA.
[Nordlund, Dennis] Stanford Linear Accelerator Ctr, Stanford Synchrotron Radiat Lightsource, Menlo Pk, CA 94025 USA.
[Lochocki, Edward B.; Shen, Kyle M.] Cornell Univ, Dept Phys, Lab Atom & Solid State Phys, Ithaca, NY 14853 USA.
[Shen, Kyle M.; Park, Jiwoong] Kavli Inst Cornell Nanoscale Sci, Ithaca, NY 14853 USA.
RP Pasupathy, AN (reprint author), Columbia Univ, Dept Phys, 538 W 120th St, New York, NY 10027 USA.
EM apn2108@columbia.edu
FU Office of Naval Research (ONR) [N00014-14-1-0501]; Air Force Office of
Scientific Research (AFOSR) [FA9550-11-1-0010]; NSF through the Cornell
Center for Materials Research (NSF) [DMR-1120296]; ONR
[N00014-12-1-0791]; AFOSR [FA9550-11-1-0033, FA2386-13-1-4118]; Nano
Material Technology Development Program through the National Research
Foundation of Korea (NRF) - Ministry of Science, ICT, and Future
Planning [2012M3A7B4049887]
FX We thank G. W. Flynn, C. Marianetti, I. L. Aleiner, B. L. Altshuler and
C. J. Arguello for helpful discussions and L. Zhao for sharing
Gr-Cu(111) bulk crystal data. This work is supported by the Office of
Naval Research (ONR) (award number N00014-14-1-0501, C.G.) and by the
Air Force Office of Scientific Research (AFOSR) (award number
FA9550-11-1-0010, A.N.P.). Work at Cornell University is supported by
the NSF through the Cornell Center for Materials Research (NSF
DMR-1120296) (J.P.). Support for synthesis and characterization was
provided by ONR (N00014-12-1-0791) (K.M.S.), AFOSR (FA9550-11-1-0033 and
FA2386-13-1-4118) (J.P.) and the Nano Material Technology Development
Program through the National Research Foundation of Korea (NRF) funded
by the Ministry of Science, ICT, and Future Planning (2012M3A7B4049887)
(J.P.). NEXAFS data was measured at beamline 8-2 at the Stanford
Synchrotron Radiation Lightsource, a National User Facility operated by
Stanford University on behalf of the US Department of Energy, Office of
Basic Energy Sciences (T.S., D.N.) and supported (T.S.) by the NSF MRSEC
Program through Columbia in the Center for Precision Assembly of
Superstratic and Superatomic Solids (DMR-1420634).
NR 38
TC 5
Z9 5
U1 1
U2 1
PU NATURE PUBLISHING GROUP
PI LONDON
PA MACMILLAN BUILDING, 4 CRINAN ST, LONDON N1 9XW, ENGLAND
SN 1745-2473
EI 1745-2481
J9 NAT PHYS
JI Nat. Phys.
PD OCT
PY 2016
VL 12
IS 10
BP 950
EP 958
DI 10.1038/NPHYS3776
PG 9
WC Physics, Multidisciplinary
SC Physics
GA DY7VP
UT WOS:000385337700019
ER
PT J
AU Lazerson, SA
Otte, M
Bozhenkov, S
Biedermann, C
Pedersen, TS
AF Lazerson, Samuel A.
Otte, Matthias
Bozhenkov, Sergey
Biedermann, Christoph
Pedersen, Thomas Sunn
CA W7-X Team
TI First measurements of error fields on W7-X using flux surface mapping(a)
SO NUCLEAR FUSION
LA English
DT Article
DE stellarator; error fields; flux surface mapping; W7-X
AB Error fields have been detected and quantified using the flux surface mapping diagnostic system on Wendelstein 7-X (W7-X). A low-field 't =1/2' magnetic configuration (t = l/2 pi), sensitive to error fields, was developed in order to detect their presence using the flux surface mapping diagnostic. In this configuration, a vacuum flux surface with rotational transform of n/m = 1/2 is created at the mid-radius of the vacuum flux surfaces. If no error fields are present a vanishingly small n/m = 5/10 island chain should be present. Modeling indicates that if an n = 1 perturbing field is applied by the trim coils, a large n/m = 1/2 island chain will be opened. This island chain is used to create a perturbation large enough to be imaged by the diagnostic. Phase and amplitude scans of the applied field allow the measurement of a small similar to 0.04 m intrinsic island chain with a 130 degrees phase relative to the first module of the W7-X experiment. These error fields are determined to be small and easily correctable by the trim coil system.
C1 [Lazerson, Samuel A.] Princeton Plasma Phys Lab, POB 451, Princeton, NJ 08543 USA.
[Otte, Matthias; Bozhenkov, Sergey; Biedermann, Christoph; Pedersen, Thomas Sunn; W7-X Team] Max Planck Inst Plasma Phys, D-17491 Greifswald, Germany.
RP Lazerson, SA (reprint author), Princeton Plasma Phys Lab, POB 451, Princeton, NJ 08543 USA.
EM lazerson@pppl.gov
OI Lazerson, Samuel/0000-0001-8002-0121
FU Euratom research and training programme [633053]
FX This work has been carried out within the framework of the EUROfusion
Consortium and has received funding from the Euratom research and
training programme 2014-2018 under grant agreement No 633053. The views
and opinions expressed herein do not necessarily reflect those of the
European Commission.
NR 20
TC 3
Z9 3
U1 1
U2 1
PU IOP PUBLISHING LTD
PI BRISTOL
PA TEMPLE CIRCUS, TEMPLE WAY, BRISTOL BS1 6BE, ENGLAND
SN 0029-5515
EI 1741-4326
J9 NUCL FUSION
JI Nucl. Fusion
PD OCT
PY 2016
VL 56
IS 10
AR 106005
DI 10.1088/0029-5515/56/10/106005
PG 11
WC Physics, Fluids & Plasmas
SC Physics
GA DW9CQ
UT WOS:000383953000009
ER
PT J
AU Gando, A
Gando, Y
Hachiya, T
Hayashi, A
Hayashida, S
Ikeda, H
Inoue, K
Ishidoshiro, K
Karino, Y
Koga, M
Matsuda, S
Mitsui, T
Nakamura, K
Obara, S
Oura, T
Ozaki, H
Shimizu, I
Shirahata, Y
Shirai, J
Suzuki, A
Takai, T
Tamae, K
Teraoka, Y
Ueshima, K
Watanabe, H
Kozlov, A
Takemoto, Y
Yoshida, S
Fushimi, K
Piepke, A
Banks, TI
Berger, BE
Fujikawa, BK
O'Donnell, T
Learned, JG
Maricic, J
Sakai, M
Winslow, LA
Krupczak, E
Ouellet, J
Efremenko, Y
Karwowski, HJ
Markoff, DM
Tornow, W
Detwiler, JA
Enomoto, S
Decowski, MP
AF Gando, A.
Gando, Y.
Hachiya, T.
Hayashi, A.
Hayashida, S.
Ikeda, H.
Inoue, K.
Ishidoshiro, K.
Karino, Y.
Koga, M.
Matsuda, S.
Mitsui, T.
Nakamura, K.
Obara, S.
Oura, T.
Ozaki, H.
Shimizu, I.
Shirahata, Y.
Shirai, J.
Suzuki, A.
Takai, T.
Tamae, K.
Teraoka, Y.
Ueshima, K.
Watanabe, H.
Kozlov, A.
Takemoto, Y.
Yoshida, S.
Fushimi, K.
Piepke, A.
Banks, T. I.
Berger, B. E.
Fujikawa, B. K.
O'Donnell, T.
Learned, J. G.
Maricic, J.
Sakai, M.
Winslow, L. A.
Krupczak, E.
Ouellet, J.
Efremenko, Y.
Karwowski, H. J.
Markoff, D. M.
Tornow, W.
Detwiler, J. A.
Enomoto, S.
Decowski, M. P.
TI A SEARCH FOR ELECTRON ANTINEUTRINOS ASSOCIATED WITH GRAVITATIONAL-WAVE
EVENTS GW150914 AND GW151226 USING KAMLAND
SO ASTROPHYSICAL JOURNAL LETTERS
LA English
DT Article
DE gravitational waves; neutrinos
ID GAMMA-RAY BURSTS; NEUTRINOS
AB We present a search, using KamLAND, a kiloton-scale anti-neutrino detector, for low-energy anti-neutrino events that were coincident with the gravitational-wave (GW) events GW150914 and GW151226, and the candidate event LVT151012. We find no inverse beta-decay neutrino events within +/-500 s of either GW signal. This non-detection is used to constrain the electron anti-neutrino fluence and the total integrated luminosity of the astrophysical sources.
C1 [Gando, A.; Gando, Y.; Hachiya, T.; Hayashi, A.; Hayashida, S.; Ikeda, H.; Inoue, K.; Ishidoshiro, K.; Karino, Y.; Koga, M.; Matsuda, S.; Mitsui, T.; Nakamura, K.; Obara, S.; Oura, T.; Ozaki, H.; Shimizu, I.; Shirahata, Y.; Shirai, J.; Suzuki, A.; Takai, T.; Tamae, K.; Teraoka, Y.; Ueshima, K.; Watanabe, H.] Tohoku Univ, Res Ctr Neutrino Sci, Sendai, Miyagi 9808578, Japan.
[Inoue, K.; Koga, M.; Nakamura, K.; Kozlov, A.; Takemoto, Y.; Piepke, A.; Berger, B. E.; Fujikawa, B. K.; Efremenko, Y.; Tornow, W.; Detwiler, J. A.; Enomoto, S.; Decowski, M. P.] Univ Tokyo, Inst Adv Study, Kavli Inst Phys & Math Universe WPI, Kashiwa, Chiba 2778583, Japan.
[Takemoto, Y.; Yoshida, S.] Osaka Univ, Grad Sch Sci, Toyonaka, Osaka 5600043, Japan.
[Fushimi, K.] Univ Tokushima, Fac Integrated Arts & Sci, Tokushima 7708502, Japan.
[Piepke, A.] Univ Alabama, Dept Phys & Astron, Tuscaloosa, AL 35487 USA.
[Banks, T. I.; O'Donnell, T.] Univ Calif Berkeley, Dept Phys, Berkeley, CA 94720 USA.
[Banks, T. I.; Berger, B. E.; Fujikawa, B. K.; O'Donnell, T.] Lawrence Berkeley Natl Lab, Berkeley, CA 94720 USA.
[Learned, J. G.; Maricic, J.; Sakai, M.] Univ Hawaii Manoa, Dept Phys & Astron, Honolulu, HI 96822 USA.
[Winslow, L. A.; Krupczak, E.; Ouellet, J.] MIT, 77 Massachusetts Ave, Cambridge, MA 02139 USA.
[Efremenko, Y.] Univ Tennessee, Dept Phys & Astron, Knoxville, TN 37996 USA.
[Efremenko, Y.] Natl Res Nucl Univ, Moscow, Russia.
[Karwowski, H. J.; Markoff, D. M.; Tornow, W.] Triangle Univ Nucl Lab, Durham, NC 27708 USA.
[Karwowski, H. J.] Univ North Carolina Chapel Hill, Chapel Hill, NC 27599 USA.
[Markoff, D. M.] North Carolina Cent Univ, Durham, NC 27701 USA.
[Tornow, W.] Duke Univ, Dept Phys, Durham, NC 27705 USA.
[Detwiler, J. A.; Enomoto, S.] Univ Washington, Ctr Expt Nucl Phys & Astrophys, Seattle, WA 98195 USA.
[Decowski, M. P.] Nikhef, Sci Pk, Amsterdam, Netherlands.
[Decowski, M. P.] Univ Amsterdam, Sci Pk, Amsterdam, Netherlands.
RP Gando, A (reprint author), Tohoku Univ, Res Ctr Neutrino Sci, Sendai, Miyagi 9808578, Japan.
FU MEXT KAKENHI Grant [26104002, 26104007]; World Premier International
Research Center Initiative (WPI Initiative), MEXT, Japan; U.S.
Department of Energy (DOE) [DE-FG03-00ER41138, DE-AC02-05CH11231,
DE-FG02-01ER41166]; DOE; NSF; Stichting Fundamenteel Onderzoek der
Materie (FOM) in the Netherlands
FX We are indebted to the LIGO Scientific Collaboration for their
gravitational-wave observations. KamLAND is supported by MEXT KAKENHI
Grant Numbers 26104002, 26104007; the World Premier International
Research Center Initiative (WPI Initiative), MEXT, Japan; and under the
U.S. Department of Energy (DOE) grants no. DE-FG03-00ER41138,
DE-AC02-05CH11231, and DE-FG02-01ER41166, as well as other DOE and NSF
grants to individual institutions, and Stichting Fundamenteel Onderzoek
der Materie (FOM) in the Netherlands. The Kamioka Mining and Smelting
Company has provided services for activities in the mine. We thank the
support of NII for SINET4.
NR 21
TC 0
Z9 0
U1 0
U2 0
PU IOP PUBLISHING LTD
PI BRISTOL
PA TEMPLE CIRCUS, TEMPLE WAY, BRISTOL BS1 6BE, ENGLAND
SN 2041-8205
EI 2041-8213
J9 ASTROPHYS J LETT
JI Astrophys. J. Lett.
PD OCT 1
PY 2016
VL 829
IS 2
AR L34
DI 10.3847/2041-8205/829/2/L34
PG 5
WC Astronomy & Astrophysics
SC Astronomy & Astrophysics
GA EJ7XG
UT WOS:000393435400001
ER
PT J
AU Seales, MB
Dilmore, R
Ertekin, T
Wang, JY
AF Seales, Maxian B.
Dilmore, Robert
Ertekin, Turgay
Wang, John Yilin
TI Numerical Analysis of the Source of Excessive Na+ and Cl- Species in
Flowback Water From Hydraulically Fractured Shale Formations
SO SPE JOURNAL
LA English
DT Article
ID DISSOLUTION KINETICS; GAS; ELECTROLYTES; MINERALS; MODEL
AB Fracture fluid is composed of fresh water, proppant, and a small percentage of other additives, which support the hydraulic-fracturing process. Excluding situations in which flowback water is recycled and reused, the total dissolved solids (TDS) in fracture fluid is limited to the fluid additives, such as potassium chloride (1 to 7 wt% KCl), which is used as a clay stabilizer to minimize clay swelling and clay-particle migration. However, the composition of recovered fluid, especially as it relates to the TDS, is always substantially different from the injected fracture fluid.
The ability to predict flowback-water volume and composition is useful when planning for the management or reuse of this aqueous byproduct stream. In this work, an ion-transport and halite-dissolution model was coupled with a fully implicit, dual-porosity, numerical simulator to study the source of the excess solutes in flowback water and to predict the concentration of both Na+ and Cl- species seen in recovered water. The results showed that mixing alone, between the injected fracture fluid and concentrated in-situ formation brine, could not account for the substantial rise in TDS seen in flowback water. Instead, the results proved that halite dissolution is a major contributor to the change in TDS seen in fracture fluid during injection and recovery. Halite dissolution can account for as much as 81% of Cl- and 86.5% of Na+ species seen in 90-day flowback water; mixing, between the injected fracture fluid and in-situ concentrated brine, accounts for approximately 19% of Cl- and 13% of Na+.
C1 [Seales, Maxian B.; Wang, John Yilin] Penn State Univ, University Pk, PA 16802 USA.
[Dilmore, Robert] Natl Energy Technol Lab, Morgantown, WV USA.
[Ertekin, Turgay] Penn State Univ, Petr & Nat Gas Engn, University Pk, PA 16802 USA.
RP Seales, MB (reprint author), Penn State Univ, University Pk, PA 16802 USA.
NR 34
TC 0
Z9 0
U1 1
U2 1
PU SOC PETROLEUM ENG
PI RICHARDSON
PA 222 PALISADES CREEK DR,, RICHARDSON, TX 75080 USA
SN 1086-055X
EI 1930-0220
J9 SPE J
JI SPE J.
PD OCT
PY 2016
VL 21
IS 5
BP 1477
EP 1490
PG 14
WC Engineering, Petroleum
SC Engineering
GA EJ6BH
UT WOS:000393303000001
ER
PT J
AU Lee, K
Moridis, GJ
Ehlig-Economides, CA
AF Lee, K.
Moridis, G. J.
Ehlig-Economides, C. A.
TI A Comprehensive Simulation Model of Kerogen Pyrolysis for the In-situ
Upgrading of Oil Shales
SO SPE JOURNAL
LA English
DT Article
ID POROUS-MEDIA; MULTIPARAMETER CORRELATION; HYDRAULIC CONDUCTIVITY;
THERMAL-CONDUCTIVITY; NUMERICAL-SIMULATION; REACTION FRONTS; EQUATION;
HYDROCARBONS; PERMEABILITY; SOLUBILITY
AB Oil shale, which is composed of abundant organic matter called kerogen, is a vast energy source. Pyrolysis of kerogen in oil shales releases recoverable hydrocarbons. Here, we describe the pyrolysis of kerogen with an in-situ upgrading process, which is applicable to the majority of oil shales. The pyrolysis is represented by six kinetic reactions resulting in 10 components and four phases. Expanding the Texas A&M Flow and Transport Simulator (FTSim), which is a variant of the TOUGH + simulator (Moridis 2014), we develop a fully functional capability that describes kerogen pyrolysis and accompanying system changes.
The simulator describes the coupled process of mass transport and heat flow through porous and fractured media and includes physical and chemical phenomena of reservoir systems. The simulator involves a total of 15 thermophysical states and all transitions between them and computes a simultaneous solution of 11 mass- and energy-balance equations per element. The simulator solves the equations in a fully implicit manner by solving Jacobian matrix equations with the Newton-Raphson iteration method. To conduct a realistic simulation, we account for geological structure of oil-shale reservoirs and physical properties of bulk-oil shale rocks by considering phases and components in the pores. In addition, we involve interaction between fluids and porous media, diverse equations of state (EOSs) for computation of fluid properties, and numerical modeling of fractured media.
We intensively reproduce the field-production data of Shell Insitu Conversion Process (ICP) implemented in the Green River formation by conducting sensitivity analyses for the diverse reservoir parameters, such as initial effective porosity of the matrix, oil-shale grade, and the spacing of the natural-fracture network. We analyze the effect of each reservoir parameter on the hydrocarbon productivity and product selectivity. The simulator provides a powerful tool to quantitatively evaluate production behavior and dynamic-system changes during in-situ upgrading of oil shales and subsequent fluid production by thoroughly describing a reservoir model, phases and components, phase behavior, phase properties, and evolution of porosity and permeability.
C1 [Lee, K.] Texas A&M Univ, College Stn, TX 77843 USA.
[Moridis, G. J.] Lawrence Berkeley Lab, Berkeley, CA USA.
[Ehlig-Economides, C. A.] Univ Houston, Houston, TX 77004 USA.
RP Lee, K (reprint author), Texas A&M Univ, College Stn, TX 77843 USA.
FU Crisman Institute for Petroleum Research at Texas AM University
FX We appreciate the Crisman Institute for Petroleum Research at Texas A&M
University for supporting this research.
NR 59
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U1 4
U2 4
PU SOC PETROLEUM ENG
PI RICHARDSON
PA 222 PALISADES CREEK DR,, RICHARDSON, TX 75080 USA
SN 1086-055X
EI 1930-0220
J9 SPE J
JI SPE J.
PD OCT
PY 2016
VL 21
IS 5
BP 1612
EP 1630
PG 19
WC Engineering, Petroleum
SC Engineering
GA EJ6BH
UT WOS:000393303000010
ER
PT J
AU Kothari, A
Charrier, M
Wu, YW
Malfatti, S
Zhou, CE
Singer, SW
Dugan, L
Mukhopadhyay, A
AF Kothari, Ankita
Charrier, Marimikel
Wu, Yu-Wei
Malfatti, Stephanie
Zhou, Carol E.
Singer, Steven W.
Dugan, Larry
Mukhopadhyay, Aindrila
TI Transcriptomic analysis of the highly efficient oil-degrading bacterium
Acinetobacter venetianus RAG-1 reveals genes important in dodecane
uptake and utilization
SO FEMS MICROBIOLOGY LETTERS
LA English
DT Article
DE alkane hydroxylase; alkane monooxygenase; dodecane; alkane uptake;
transcriptomic; Acinetobacter venetianus RAG-1 ATCC 31012
ID INDOLEPYRUVATE FERREDOXIN OXIDOREDUCTASE; ALKANE HYDROXYLASES;
ESCHERICHIA-COLI; N-ALKANES; DIFFERENTIAL EXPRESSION;
ALCANIVORAX-BORKUMENSIS; PSEUDOMONAS-AERUGINOSA; METABOLIC ADAPTATIONS;
SUBSYSTEMS TECHNOLOGY; CALCOACETICUS RAG-1
AB The hydrocarbonoclastic bacterium Acinetobacter venetianus RAG-1 has attracted substantial attention due to its powerful oil-degrading capabilities and its potential to play an important ecological role in the cleanup of alkanes. In this study, we compare the transcriptome of the strain RAG-1 grown in dodecane, the corresponding alkanol (dodecanol), and sodium acetate for the characterization of genes involved in dodecane uptake and utilization. Comparison of the transcriptional responses of RAG-1 grown on dodecane led to the identification of 1074 genes that were differentially expressed relative to sodium acetate. Of these, 622 genes were upregulated when grown in dodecane. The highly upregulated genes were involved in alkane catabolism, along with stress response. Our data suggest AlkMb to be primarily involved in dodecane oxidation. Transcriptional response of RAG-1 grown on dodecane relative to dodecanol also led to the identification of permease, outer membrane protein and thin fimbriae coding genes potentially involved in dodecane uptake. This study provides the first model for key genes involved in alkane uptake and metabolism in A. venetianus RAG-1.
C1 [Kothari, Ankita; Charrier, Marimikel; Wu, Yu-Wei; Singer, Steven W.; Mukhopadhyay, Aindrila] Lawrence Berkeley Natl Lab, Biol Syst & Engn, Berkeley, CA 94720 USA.
[Wu, Yu-Wei; Dugan, Larry] Taipei Med Univ, Grad Inst Biomed Informat, Taiwan Biosci, Taipei 110, Taiwan.
[Malfatti, Stephanie; Dugan, Larry] Lawrence Livermore Natl Lab, Div Biotechnol, Livermore, CA 94550 USA.
[Zhou, Carol E.] Lawrence Livermore Natl Lab, Comp Applicat & Res Dept, Livermore, CA 94550 USA.
RP Mukhopadhyay, A (reprint author), Lawrence Berkeley Natl Lab, Biol Syst & Engn, Berkeley, CA 94720 USA.
EM amukhopadhyay@lbl.gov
FU Lawrence Livermore National Lab (LLNL) via US Department of Energy,
Office of Science, Office of Biological and Environmental Research
[DE-AC02-05CH11231, IC009952, B604346, YN1901000]; US Department of
Energy by LLNL [DE-AC52-07NA27344]
FX This work was supported by funding from the Lawrence Livermore National
Lab (LLNL) via US Department of Energy, Office of Science, Office of
Biological and Environmental Research Contract DE-AC02-05CH11231 between
Lawrence Berkeley National Laboratory and the US Department of Energy
[LBNL Award No.: IC009952, Sponsor Award No.: B604346, WFO B&R Code:
YN1901000]. This work was performed under the auspices of the US
Department of Energy by LLNL under Contract DE-AC52-07NA27344. The US
Government retains and the publisher, by accepting the article for
publication, acknowledges that the US Government retains a
non-exclusive, paid-up, irrevocable, worldwide license to publish or
reproduce the published form of this manuscript, or allow others to do
so, for US Government purposes.
NR 55
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U1 3
U2 3
PU OXFORD UNIV PRESS
PI OXFORD
PA GREAT CLARENDON ST, OXFORD OX2 6DP, ENGLAND
SN 0378-1097
EI 1574-6968
J9 FEMS MICROBIOL LETT
JI FEMS Microbiol. Lett.
PD OCT
PY 2016
VL 363
IS 20
AR fnw224
DI 10.1093/femsle/fnw224
PG 9
WC Microbiology
SC Microbiology
GA EI8HL
UT WOS:000392746700004
ER
PT J
AU Yan, JP
Joshee, N
Liu, SJ
AF Yan, Jipeng
Joshee, Nirmal
Liu, Shijie
TI Utilization of Hardwood in Biorefinery: A Kinetic Interpretation of
Pilot-Scale Hot-Water Pretreatment of Paulownia elongata Woodchips
SO Journal of Biobased Materials and Bioenergy
LA English
DT Article
DE Hot-Water Extraction; Kinetics; Paulownia elongata; Glucose;
Xylooligomers
ID WOODY BIOMASS; ETHANOL-PRODUCTION; SUGAR MAPLE; AUTOHYDROLYSIS;
HYDROLYSIS; EXTRACTION; ENERGY; XYLAN; TECHNOLOGY; OLIGOSACCHARIDES
AB Hot water extraction of summer-harvested Paulownia elongata in a pilot-scale reactor of 1.84 m(3) was investigated at 160 degrees C for 2.5 h. Monomeric sugars, carboxylic acids, and xylo-oligomers were the major components in the hot water extract. Unlike the extraction results of fall/winter harvested Paulownia elongata, glucose was the dominant monosaccharide in the extraction liquor especially during early stage of the extraction of the wood harvested during active growth in summer. The maximum concentration of glucose recorded was 0.013 mol/L. The xylo-oligomers concentration, reaching up to 0.012 mol/L, were the main oligosaccharides. Concentrations of furfural and hydroxymethylfurfural (HMF) increased with extraction time and reached a maximum value of 0.0053 mol/L and 0.004 mol/L, respectively, by the end of extraction. Pseudo-zeroth order rate kinetic models were employed to describe the change in dissolved solids, xylooligomer, monomer sugars, acids, furfural, and HMF in the hot water extract.
C1 [Yan, Jipeng; Liu, Shijie] SUNY Coll Environm Sci & Forestry, Dept Paper & Bioproc Engn, 1 Forestry Dr, Syracuse, NY 13210 USA.
[Yan, Jipeng] Lawrence Berkeley Natl Lab, Adv Biofuels & Bioprod Proc Demonstrat Unit, Emeryville, CA USA.
[Joshee, Nirmal] Ft Valley State Univ, Agr Res Stn, 1005 State Univ Dr, Ft Valley, GA 31030 USA.
RP Liu, SJ (reprint author), SUNY Coll Environm Sci & Forestry, Dept Paper & Bioproc Engn, 1 Forestry Dr, Syracuse, NY 13210 USA.
EM sliu@esf.edu
FU Biorefinery and Bioprocess Engineering Research group at the SUNY ESF;
CSREES [2014-01293]; USDA NIFA
FX The authors appreciate the support from Biorefinery and Bioprocess
Engineering Research group at the SUNY ESF. In addition, the authors are
grateful to the help of Yipeng Xie and Christopher D. Wood. N. Joshee
would like to thank USDA NIFA for-Capacity building grant "Developing a
sustainable bioenergy system: Paulownia production for fuel, chemicals,
and materials" (2013-2016). CSREES Award #2014-01293, (P.I.: Nirmal
Joshee; S. Liu, Co-PI).
NR 51
TC 3
Z9 3
U1 6
U2 6
PU AMER SCIENTIFIC PUBLISHERS
PI VALENCIA
PA 26650 THE OLD RD, STE 208, VALENCIA, CA 91381-0751 USA
SN 1556-6560
EI 1556-6579
J9 J BIOBASED MATER BIO
JI J. Biobased Mater. Bioenergy
PD OCT
PY 2016
VL 10
IS 5
BP 339
EP 348
DI 10.1166/jbmb.2016.1609
PG 10
WC Chemistry, Applied; Energy & Fuels; Materials Science, Biomaterials
SC Chemistry; Energy & Fuels; Materials Science
GA EJ0CS
UT WOS:000392876800003
ER
PT J
AU Adam, R
Ade, PAR
Aghanim, N
Arnaud, M
Ashdown, M
Aumont, J
Baccigalupi, C
Banday, AJ
Barreiro, RB
Bartolo, N
Battaner, E
Benabed, K
Benoit, A
Benoit-Levy, A
Bernard, JP
Bersanelli, M
Bertincourt, B
Bielewicz, P
Bock, JJ
Bonavera, L
Bond, JR
Borrill, J
Bouchet, FR
Boulanger, F
Bucher, M
Burigana, C
Calabrese, E
Cardoso, JF
Catalano, A
Challinor, A
Chamballu, A
Chary, RR
Chiang, HC
Christensen, PR
Clements, DL
Colombi, S
Colombo, LPL
Combet, C
Couchot, F
Coulais, A
Crill, BP
Curto, A
Cuttaia, F
Danese, L
Davies, RD
Davis, RJ
de Bernardis, P
de Rosa, A
de Zotti, G
Delabrouille, J
Delouis, JM
Desert, FX
Diego, JM
Dole, H
Donzelli, S
Dure, O
Douspis, M
Ducout, A
Dupac, X
Efstathiou, G
Elsner, F
Ensslin, TA
Eriksen, HK
Falgarone, E
Fergusson, J
Finelli, F
Forni, O
Frailis, M
Fraisse, AA
Franceschi, E
Frejser, A
Galeotta, S
Galli, S
Ganga, K
Ghosh, T
Giard, M
Giraud-Heraudl, Y
Gjerlow, E
Gonzalez-Nuevo, J
Gorski, KM
Gratton, S
Gruppuso, A
Gudmundsson, JE
Hansen, FK
Hanson, D
Harrison, DL
Henrot-Versille, S
Herranz, D
Hildebrandt, SR
Hivon, E
Hobson, M
Holmes, WA
Hornstrup, A
Hovest, W
Huffenberger, KM
Hurier, G
Jaffe, AH
Jaffe, TR
Jones, WC
Juvela, M
Keihanen, E
Keskitalo, R
Kisner, TS
Kneissl, R
Knoche, J
Kunz, M
Kurki-Suonio, H
Lagache, G
Lamarre, JM
Lasenby, A
Lattanzi, M
Lawrence, CR
Le Jenne, M
Leahy, JP
Lellouch, E
Leonardi, R
Lesgourgues, J
Levrier, F
Liguori, M
Lilje, PB
Linden-Vornle, M
Lopez-Caniego, M
Lubin, PM
Macias-Perez, JF
Maggie, G
Maino', D
Mandolesi, N
Mangilli, A
Maris, M
Martin, PG
Martinez-Gonzalez, E
Masi, S
Matarrese, S
McGehee, P
Melchiorri, A
Mendes, L
Mennella, A
Migliaccio, M
Mitra, S
Miville-Deschenes, MA
Moneti, A
Montier, L
Moreno, R
Morgante, G
Mortlock, D
Moss, A
Mottet, S
Munshi, D
Murphy, JA
Naselsky, P
Nati, F
Natoli, P
Netterfield, CB
Norgaard-Nielsen, HU
Noviello, F
Novikov, D
Novikov, I
Oxborrow, CA
Paci, F
Pagano, L
Pajot, F
Paoletti, D
Pasian, F
Patanchon, G
Pearson, TJ
Perdereau, O
Perotto, L
Perrotta, F
Pettorino, V
Piacentini, F
Piat, M
Pierpaoli, E
Pietrobon, D
Plaszczynski, S
Pointecouteau, E
Polenta, G
Pratt, GW
Prezeau, G
Prunet, S
Puget, JL
Rachen, JP
Reinecke, M
Remazeilles, M
Renault, C
Renzi, A
Ristorcelli, I
Rocha, G
Rosset, C
Rossetti, M
Roudier, G
Rowan-Robinson, M
Rusholme, B
Sandri, M
Santos, D
Sauve, A
Savelainen, M
Savini, G
Scott, D
Seiffert, MD
Shellard, EPS
Spencer, LD
Stolyarov, V
Stompor, R
Sudiwala, R
Sutton, D
Suur-Uski, AS
Sygnet, JF
Tauber, JA
Terenzi, L
Toffolatti, L
Tomasi, M
Tristram, M
Tucci, M
Tuovinen, J
Valenziano, L
Valiviita, J
Van Tent, B
Vibert, L
Vielva, P
Villa, F
Wade, LA
Wandelt, BD
Watson, R
Wehus, IK
Yvon, D
Zacchei, A
Zonca, A
AF Adam, R.
Ade, P. A. R.
Aghanim, N.
Arnaud, M.
Ashdown, M.
Aumont, J.
Baccigalupi, C.
Banday, A. J.
Barreiro, R. B.
Bartolo, N.
Battaner, E.
Benabed, K.
Benoit, A.
Benoit-Levy, A.
Bernard, J. -P.
Bersanelli, M.
Bertincourt, B.
Bielewicz, P.
Bock, J. J.
Bonavera, L.
Bond, J. R.
Borrill, J.
Bouchet, F. R.
Boulanger, F.
Bucher, M.
Burigana, C.
Calabrese, E.
Cardoso, J. -F.
Catalano, A.
Challinor, A.
Chamballu, A.
Chary, R. -R.
Chiang, H. C.
Christensen, P. R.
Clements, D. L.
Colombi, S.
Colombo, L. P. L.
Combet, C.
Couchot, F.
Coulais, A.
Crill, B. P.
Curto, A.
Cuttaia, F.
Danese, L.
Davies, R. D.
Davis, R. J.
de Bernardis, P.
de Rosa, A.
de Zotti, G.
Delabrouille, J.
Delouis, J. -M.
Desert, F. -X.
Diego, J. M.
Dole, H.
Donzelli, S.
Dure, O.
Douspis, M.
Ducout, A.
Dupac, X.
Efstathiou, G.
Elsner, F.
Ensslin, T. A.
Eriksen, H. K.
Falgarone, E.
Fergusson, J.
Finelli, F.
Forni, O.
Frailis, M.
Fraisse, A. A.
Franceschi, E.
Frejser, A.
Galeotta, S.
Galli, S.
Ganga, K.
Ghosh, T.
Giard, M.
Giraud-Heraudl, Y.
Gjerlow, E.
Gonzalez-Nuevo, J.
Gorski, K. M.
Gratton, S.
Gruppuso, A.
Gudmundsson, J. E.
Hansen, F. K.
Hanson, D.
Harrison, D. L.
Henrot-Versille, S.
Herranz, D.
Hildebrandt, S. R.
Hivon, E.
Hobson, M.
Holmes, W. A.
Hornstrup, A.
Hovest, W.
Huffenberger, K. M.
Hurier, G.
Jaffe, A. H.
Jaffe, T. R.
Jones, W. C.
Juvela, M.
Keihanen, E.
Keskitalo, R.
Kisner, T. S.
Kneissl, R.
Knoche, J.
Kunz, M.
Kurki-Suonio, H.
Lagache, G.
Lamarre, J. -M.
Lasenby, A.
Lattanzi, M.
Lawrence, C. R.
Le Jenne, M.
Leahy, J. P.
Lellouch, E.
Leonardi, R.
Lesgourgues, J.
Levrier, F.
Liguori, M.
Lilje, P. B.
Linden-Vornle, M.
Lopez-Caniego, M.
Lubin, P. M.
Macias-Perez, J. F.
Maggie, G.
Maino', D.
Mandolesi, N.
Mangilli, A.
Maris, M.
Martin, P. G.
Martinez-Gonzalez, E.
Masi, S.
Matarrese, S.
McGehee, P.
Melchiorri, A.
Mendes, L.
Mennella, A.
Migliaccio, M.
Mitra, S.
Miville-Deschenes, M. -A.
Moneti, A.
Montier, L.
Moreno, R.
Morgante, G.
Mortlock, D.
Moss, A.
Mottet, S.
Munshi, D.
Murphy, J. A.
Naselsky, P.
Nati, F.
Natoli, P.
Netterfield, C. B.
Norgaard-Nielsen, H. U.
Noviello, F.
Novikov, D.
Novikov, I.
Oxborrow, C. A.
Paci, F.
Pagano, L.
Pajot, F.
Paoletti, D.
Pasian, F.
Patanchon, G.
Pearson, T. J.
Perdereau, O.
Perotto, L.
Perrotta, F.
Pettorino, V.
Piacentini, F.
Piat, M.
Pierpaoli, E.
Pietrobon, D.
Plaszczynski, S.
Pointecouteau, E.
Polenta, G.
Pratt, G. W.
Prezeau, G.
Prunet, S.
Puget, J. -L.
Rachen, J. P.
Reinecke, M.
Remazeilles, M.
Renault, C.
Renzi, A.
Ristorcelli, I.
Rocha, G.
Rosset, C.
Rossetti, M.
Roudier, G.
Rowan-Robinson, M.
Rusholme, B.
Sandri, M.
Santos, D.
Sauve, A.
Savelainen, M.
Savini, G.
Scott, D.
Seiffert, M. D.
Shellard, E. P. S.
Spencer, L. D.
Stolyarov, V.
Stompor, R.
Sudiwala, R.
Sutton, D.
Suur-Uski, A. -S.
Sygnet, J. -F.
Tauber, J. A.
Terenzi, L.
Toffolatti, L.
Tomasi, M.
Tristram, M.
Tucci, M.
Tuovinen, J.
Valenziano, L.
Valiviita, J.
Van Tent, B.
Vibert, L.
Vielva, P.
Villa, F.
Wade, L. A.
Wandelt, B. D.
Watson, R.
Wehus, I. K.
Yvon, D.
Zacchei, A.
Zonca, A.
CA Planck Collaboration
TI Planck 2015 results VII. High Frequency Instrument data processing:
Time-ordered information and beams
SO ASTRONOMY & ASTROPHYSICS
LA English
DT Article
DE methods: data analysis; cosmic background radiation; instrumentation:
detectors
ID PRE-LAUNCH STATUS
AB The Planck High Frequency Instrument (HFI) has observed the full sky at six frequencies (100, 143, 217, 353, 545, and 857 GHz) in intensity and at four frequencies in linear polarization (100, 143, 217, and 353 GHz). In order to obtain sky maps, the time-ordered information (TOI) containing the detector and pointing samples must be processed and the angular response must be assessed. The full mission TOI is included in the Planck 2015 release. This paper describes the HFI TOI and beam processing for the 2015 release. HFI calibration and map making are described in a companion paper. The main pipeline has been modified since the last release (2013 nominal mission in intensity only), by including a correction for the nonlinearity of the warm readout and by improving the model of the bolometer time response. The beam processing is an essential tool that derives the angular response used in all the Planck science papers and we report an improvement in the effective beam window function uncertainty of more than a factor of 10 relative to the 2013 release. Noise correlations introduced by pipeline filtering function are assessed using dedicated simulations. Angular cross-power spectra using data sets that are decorrelated in time are immune to the main systematic effects.
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[Kunz, M.] African Inst Math Sci, 6-8 Melrose Rd, ZA-7945 Cape Town, South Africa.
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[Lagache, G.] Aix Marseille Univ, CNRS, LAM, UMR 7326, F-13388 Marseille, France.
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[Tuovinen, J.] Trinity Coll Dublin, CRANN, Dublin, Ireland.
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[Huffenberger, K. M.] Florida State Univ, Dept Phys, Keen Phys Bldg,77 Chieftan Way, Tallahassee, FL 32306 USA.
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[Bersanelli, M.; Maino', D.; Mennella, A.; Rossetti, M.; Tomasi, M.] Univ Milan, Dipartimento Fis, Via Celoria 16, I-20122 Milan, Italy.
[Renzi, A.] Univ Roma Tor Vergata, Dipartimento Matemat, Via Ric Sci 1, Rome, Italy.
[Christensen, P. R.; Naselsky, P.] Niels Bohr Inst, Discovery Ctr, 17 Blegdamsvej, Copenhagen, Denmark.
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[Remazeilles, M.; Tauber, J. A.] European Space Agcy, Estec, Keplerlaan 1, NL-2201 AZ Noordwijk, Netherlands.
[Terenzi, L.] Univ E Campus, Fac Ingn, Via Isimbardi 10, I-22060 Novedrate, CO, Italy.
[Matarrese, S.] Ist Nazl Fis Nucl, Gran Sasso Sci Inst, Viale F Crispi 7, I-67100 Laquila, Italy.
[Pettorino, V.; Pointecouteau, E.] HGSFP, Philosophenweg 16, D-69120 Heidelberg, Germany.
[Pettorino, V.; Pointecouteau, E.] Heidelberg Univ, Dept Theoret Phys, Philosophenweg 16, D-69120 Heidelberg, Germany.
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[de Zotti, G.] INAF Osservatorio Astron Padova, Vicolo Osservatorio 5, I-35141 Padua, Italy.
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[Burigana, C.; Cuttaia, F.; de Rosa, A.; Finelli, F.; Franceschi, E.; Gruppuso, A.; Mandolesi, N.; Morgante, G.; Natoli, P.; Paoletti, D.; Sandri, M.; Terenzi, L.; Toffolatti, L.; Valenziano, L.; Villa, F.] INAF IASF Bologna, Via Gobetti 101, I-40147 Bologna, Italy.
[Bersanelli, M.; Donzelli, S.; Maino', D.; Mennella, A.; Rossetti, M.; Tomasi, M.] INAF IASF Milano, Via E Bassini 15, I-20133 Milan, Italy.
[Burigana, C.; Finelli, F.; Paoletti, D.] Ist Nazl Fis Nucl, Sez Bologna, Via Irnerio 46, I-40126 Bologna, Italy.
[Melchiorri, A.; Pagano, L.] Univ Roma Sapienza, Sez Roma 1, Ist Nazl Fis Nucl, Piazzale Aldo Moro 2, I-00185 Rome, Italy.
[Renzi, A.] Univ Roma Tor Vergata, Sez Roma 2, Ist Nazl Fis Nucl, Via Ric Sci 1, Rome, Italy.
[Desert, F. -X.] Univ Grenoble Alpes, IPAG, CNRS, F-38000 Grenoble, France.
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[Clements, D. L.; Ducout, A.; Jaffe, A. H.; Mortlock, D.; Rowan-Robinson, M.] Imperial Coll London, Astrophys Grp, Blackett Lab, Prince Consort Rd, London SW7 2AZ, England.
[Chary, R. -R.; McGehee, P.; Pearson, T. J.; Rusholme, B.] CALTECH, Infrared Proc & Anal Ctr, Pasadena, CA 91125 USA.
[Benoit, A.] Univ Joseph Fourier Grenoble I, Inst Neel, CNRS, 25 Rue Martyrs, F-38042 Grenoble, France.
[Dole, H.] Inst Univ France, 103 Bd St Michel, F-75005 Paris, France.
[Aghanim, N.; Aumont, J.; Bertincourt, B.; Boulanger, F.; Chamballu, A.; Dole, H.; Douspis, M.; Ghosh, T.; Hurier, G.; Kunz, M.; Lagache, G.; Mangilli, A.; Miville-Deschenes, M. -A.; Pajot, F.; Puget, J. -L.; Remazeilles, M.; Vibert, L.] Univ Paris Sud 11, CNRS, Inst Astrophys Spatiale, UMR 8617, Batiment 121, F-91400 Orsay, France.
[Benabed, K.; Benoit-Levy, A.; Bouchet, F. R.; Cardoso, J. -F.; Colombi, S.; Delouis, J. -M.; Ducout, A.; Elsner, F.; Hivon, E.; Moneti, A.; Mottet, S.; Prunet, S.; Sygnet, J. -F.; Wandelt, B. D.] Inst Astrophys Paris, CNRS, UMR 7095, 98 Bis Blvd Arago, F-75014 Paris, France.
[Lesgourgues, J.] Rhein Westfal TH Aachen, Inst Theoret Teilchenphys & Kosmol, D-52056 Aachen, Germany.
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[Eriksen, H. K.; Gjerlow, E.; Hansen, F. K.; Lilje, P. B.] Univ Oslo, Inst Theoret Astrophys, Oslo, Norway.
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[Bartolo, N.; Liguori, M.; Matarrese, S.] Ist Nazl Fis Nucl, Sez Padova, Via Marzolo 8, I-35131 Padua, Italy.
[Bock, J. J.; Colombo, L. P. L.; Crill, B. P.; Dure, O.; Gorski, K. M.; Hanson, D.; Hildebrandt, S. R.; Holmes, W. A.; Lawrence, C. R.; Mitra, S.; Pietrobon, D.; Prezeau, G.; Rocha, G.; Roudier, G.; Seiffert, M. D.; Wade, L. A.; Wehus, I. K.] CALTECH, Jet Prop Lab, 4800 Oak Grove Dr, Pasadena, CA USA.
[Davies, R. D.; Davis, R. J.; Leahy, J. P.; Noviello, F.; Watson, R.] Univ Manchester, Jodrell Bank Ctr Astrophys, Sch Phys & Astron, Alan Turing Bldg,Oxford Rd, Manchester M13 9PL, Lancs, England.
[Galli, S.] Univ Chicago, Kavli Inst Cosmol Phys, Chicago, IL 60637 USA.
[Ashdown, M.; Challinor, A.; Curto, A.; Gratton, S.; Harrison, D. L.; Lasenby, A.; Migliaccio, M.; Stolyarov, V.; Sutton, D.] Kavli Inst Cosmol Cambridge, Madingley Rd, Cambridge CB3 0HA, England.
[Couchot, F.; Henrot-Versille, S.; Mangilli, A.; Moreno, R.; Perdereau, O.; Plaszczynski, S.; Tristram, M.] Univ Paris 11, LAL, CNRS IN2P3, F-91400 Orsay, France.
[Catalano, A.; Coulais, A.; Falgarone, E.; Lamarre, J. -M.; Levrier, F.; Roudier, G.] CNRS, LERMA, 61 Ave Observ, F-75014 Paris, France.
[Lellouch, E.; Moreno, R.] Univ Paris Diderot, CNRS, LESIA, Observ Paris, 5 Pl J Janssen, F-92195 Meudon, France.
[Arnaud, M.; Chamballu, A.; Pratt, G. W.] Univ Paris Diderot, Lab AIM, IRFU Serv Astrophys, CEA DSM,CNRS,CEA Saclay, Bat 709, F-91191 Gif Sur Yvette, France.
[Cardoso, J. -F.] CNRS, Lab Traitement & Commun Informat, UMR 5141, 46 Rue Barrault, F-75634 Paris 13, France.
[Adam, R.; Catalano, A.; Combet, C.; Macias-Perez, J. F.; Perotto, L.; Renault, C.; Santos, D.] Univ Grenoble Alpes, CNRS IN2P3, Lab Phys Subat & Cosmol, 53 Rue Martyrs, F-38026 Grenoble, France.
[Van Tent, B.] Univ Paris Sud 11, Lab Phys Theor, Batiment 210, F-91405 Orsay, France.
[Van Tent, B.] CNRS, Batiment 210, F-91405 Orsay, France.
[Kisner, T. S.] Lawrence Berkeley Natl Lab, Berkeley, CA 94720 USA.
[Novikov, D.; Novikov, I.] Russian Acad Sci, Lebedev Phys Inst, Ctr Astro Space, 84-32 Profsoyuznaya St,GSP 7, Moscow 117997, Russia.
[Ensslin, T. A.; Hovest, W.; Knoche, J.; Rachen, J. P.; Reinecke, M.] Max Planck Inst Astrophys, Karl Schwarzschild Str 1, D-85741 Garching, Germany.
[Hanson, D.] McGill Univ, McGill Phys, Ernest Rutherford Phys Bldg,3600 Rue Univ, Montreal, PQ H3A 2T8, Canada.
[Murphy, J. A.] Natl Univ Ireland, Dept Expt Phys, Maynooth, Kildare, Ireland.
[Bielewicz, P.] Nicolaus Copernicus Astron Ctr, Bartycka 18, PL-00716 Warsaw, Poland.
[Christensen, P. R.; Frejser, A.; Naselsky, P.; Novikov, I.] Niels Bohr Inst, Blegdamsvej 17, DK-2100 Copenhagen, Denmark.
[Savini, G.] UCL, Opt Sci Lab, Gower St, London WC1E 6BT, England.
[Baccigalupi, C.; Bielewicz, P.; Danese, L.; de Zotti, G.; Paci, F.; Perrotta, F.] SISSA, Astrophys Sect, Via Bonomea 265, I-34136 Trieste, Italy.
[Ade, P. A. R.; Munshi, D.; Spencer, L. D.; Sudiwala, R.] Cardiff Univ, Sch Phys & Astron, Queens Bldg, Cardiff CF24 3AA, Wales.
[Moss, A.] Univ Nottingham, Sch Phys & Astron, Nottingham NG7 2RD, England.
[Bouchet, F. R.] Sorbonne Univ UPMC, UMR 7095, Inst Astrophys Paris, 98 Bis Blvd Arago, F-75014 Paris, France.
[Borrill, J.] Univ Calif Berkeley, Space Sci Lab, Berkeley, CA 94720 USA.
[Stolyarov, V.] Russian Acad Sci, Special Astrophys Observ, Karachai Cherkessian Rep 369167, Zelenchukskiy R, Russia.
[Calabrese, E.] Univ Oxford, Subdept Astrophys, Oxford OX1 3RH, England.
[Lesgourgues, J.] CERN, Div Theory, PH TH, CH-1211 Geneva 23, Switzerland.
[Benabed, K.; Benoit-Levy, A.; Colombi, S.; Delouis, J. -M.; Elsner, F.; Hivon, E.; Prunet, S.; Wandelt, B. D.] UPMC Univ Paris 06, UMR 7095, 98 Bis Blvd Arago, F-75014 Paris, France.
[Banday, A. J.; Bernard, J. -P.; Forni, O.; Giard, M.; Jaffe, T. R.; Montier, L.; Pointecouteau, E.; Ristorcelli, I.; Sauve, A.] Univ Toulouse, UPS OMP, IRAP, F-31028 Toulouse 4, France.
[Battaner, E.] Univ Granada, Fac Ciencias, Dept Fis Teor & Cosmos, E-18071 Granada, Spain.
[Battaner, E.] Univ Granada, Inst Carlos Fis Teor & Computac 1, Granada 18071, Spain.
[Gorski, K. M.] Univ Warsaw Observ, Aleje Ujazdowskie 4, PL-00478 Warsaw, Poland.
RP Crill, BP (reprint author), CALTECH, Pasadena, CA 91125 USA.; Desert, FX (reprint author), Univ Grenoble Alpes, IPAG, CNRS, F-38000 Grenoble, France.; Crill, BP (reprint author), CALTECH, Jet Prop Lab, 4800 Oak Grove Dr, Pasadena, CA USA.
EM bcrill@jpl.nasa.gov; francois-xavier.desert@obs.ujf-grenoble.fr
RI Barreiro, Rita Belen/N-5442-2014; bonavera, laura/E-9368-2017;
Gonzalez-Nuevo, Joaquin/I-3562-2014; Herranz, Diego/K-9143-2014;
Colombo, Loris/J-2415-2016;
OI Lilje, Per/0000-0003-4324-7794; Nati, Federico/0000-0002-8307-5088;
Savini, Giorgio/0000-0003-4449-9416; Pierpaoli,
Elena/0000-0002-7957-8993; Watson, Robert/0000-0002-5873-0124;
Toffolatti, Luigi/0000-0003-2645-7386; Barreiro, Rita
Belen/0000-0002-6139-4272; bonavera, laura/0000-0001-8039-3876;
Gonzalez-Nuevo, Joaquin/0000-0003-1354-6822; Herranz,
Diego/0000-0003-4540-1417; Colombo, Loris/0000-0003-4572-7732; Villa,
Fabrizio/0000-0003-1798-861X; Zacchei, Andrea/0000-0003-0396-1192;
Stolyarov, Vladislav/0000-0001-8151-828X; Paoletti,
Daniela/0000-0003-4761-6147; TERENZI, LUCA/0000-0001-9915-6379;
Valiviita, Jussi/0000-0001-6225-3693
FU ESA; CNES (France); CNRS/INSU-IN2P3-INP (France); ASI (Italy); CNR
(Italy); INAF (Italy); NASA (USA); DoE (USA); STFC (UK); UKSA (UK); CSIC
(Spain); MINECO (Spain); JA (Spain); RES (Spain); Tekes (Finland); AoF
(Finland); CSC (Finland); DLR (Germany); MPG (Germany); CSA (Canada);
DTU Space (Denmark); SER/SSO (Switzerland); RCN (Norway); SFI (Ireland);
FCT/MCTES (Portugal); ERC (EU); PRACE (EU)
FX The Planck Collaboration acknowledges the support of: ESA; CNES and
CNRS/INSU-IN2P3-INP (France); ASI, CNR, and INAF (Italy); NASA and DoE
(USA); STFC and UKSA (UK); CSIC, MINECO, JA, and RES (Spain); Tekes,
AoF, and CSC (Finland); DLR and MPG (Germany); CSA (Canada); DTU Space
(Denmark); SER/SSO (Switzerland); RCN (Norway); SFI (Ireland); FCT/MCTES
(Portugal); ERC and PRACE (EU). A description of the Planck
Collaboration and a list of its members, indicating which technical or
scientific activities they have been involved in, can be found at
http://www.cosmos.esa.int/web/planck/planck-collaboration.
NR 53
TC 0
Z9 0
U1 0
U2 0
PU EDP SCIENCES S A
PI LES ULIS CEDEX A
PA 17, AVE DU HOGGAR, PA COURTABOEUF, BP 112, F-91944 LES ULIS CEDEX A,
FRANCE
SN 1432-0746
J9 ASTRON ASTROPHYS
JI Astron. Astrophys.
PD OCT
PY 2016
VL 594
AR A7
DI 10.1051/0004-6361/201525844
PG 30
WC Astronomy & Astrophysics
SC Astronomy & Astrophysics
GA DZ4MG
UT WOS:000385832200017
ER
PT J
AU Adam, R
Ade, PAR
Aghanim, N
Arnaud, M
Ashdown, M
Aumont, J
Baccigalupi, C
Banday, AJ
Barreiro, RB
Bartolo, N
Battaner, E
Benabed, K
Benoit, A
Benoit-Levy, A
Bernard, JP
Bersanelli, M
Bertincourt, B
Bielewicz, P
Bock, JJ
Bonavera, L
Bond, JR
Borrill, J
Bouchet, FR
Boulanger, F
Bucher, M
Burigana, C
Calabrese, E
Cardoso, JF
Catalano, A
Challinor, A
Chamballu, A
Chiang, HC
Christensen, PR
Clements, DL
Colombi, S
Colombo, LPL
Combet, C
Couchot, F
Coulais, A
Crill, BP
Curto, A
Cuttaia, F
Danese, L
Davies, RD
Davis, RJ
de Bernardis, P
de Rosa, A
de Zotti, G
Delabrouille, J
Delouis, JM
Desert, FX
Diego, JM
Dole, H
Donzelli, S
Dore, O
Douspis, M
Ducout, A
Dupac, X
Efstathiou, G
Elsner, F
Ensslin, TA
Eriksen, HK
Falgarone, E
Fergusson, J
Finelli, F
Forni, O
Frailis, M
Fraisse, AA
Franceschi, E
Frejsel, A
Galeotta, S
Galli, S
Ganga, K
Ghosh, T
Giard, M
Giraud-Heraud, Y
Gjerlow, E
Gonzalez-Nuevo, J
Gorski, KM
Gratton, S
Gruppuso, A
Gudmundsson, JE
Hansen, FK
Hanson, D
Harrison, DL
Henrot-Versille, S
Herranz, D
Hildebrandt, SR
Hivon, E
Hobson, M
Holmes, WA
Hornstrup, A
Hovest, W
Huffenberger, KM
Hurier, G
Jaffe, AH
Jaffe, TR
Jones, WC
Juvela, M
Keihanen, E
Keskitalo, R
Kisner, TS
Kneissl, R
Knoche, J
Kunz, M
Kurki-Suonio, H
Lagache, G
Lamarre, JM
Lasenby, A
Lattanzi, M
Lawrence, CR
Le Jeune, M
Leahy, JP
Lellouch, E
Leonardi, R
Lesgourgues, J
Levrier, F
Liguori, M
Lilje, PB
Linden-Vornle, M
Lopez-Caniego, M
Lubin, PM
Macias-Perez, JF
Maggio, G
Maino, D
Mandolesi, N
Mangilli, A
Maris, M
Martin, PG
Martinez-Gonzalez, E
Masi, S
Matarrese, S
McGehee, P
Melchiorri, A
Mendes, L
Mennella, A
Migliaccio, M
Mitra, S
Miville-Deschenes, MA
Moneti, A
Montier, L
Moreno, R
Morgante, G
Mortlock, D
Moss, A
Mottet, S
Munshi, D
Murphy, JA
Naselsky, P
Nati, F
Natoli, P
Netterfield, CB
Norgaard-Nielsen, HU
Noviello, F
Novikov, D
Novikov, I
Oxborrow, CA
Paci, F
Pagano, L
Pajot, F
Paoletti, D
Pasian, F
Patanchon, G
Pearson, TJ
Perdereau, O
Perotto, L
Perrotta, F
Pettorino, V
Piacentini, F
Piat, M
Pierpaoli, E
Pietrobon, D
Plaszczynski, S
Pointecouteau, E
Polenta, G
Pratt, GW
Prezeau, G
Prunet, S
Puget, JL
Rachen, JP
Reinecke, M
Remazeilles, M
Renault, C
Renzi, A
Ristorcelli, I
Rocha, G
Rosset, C
Rossetti, M
Roudier, G
Rusholme, B
Sandri, M
Santos, D
Sauve, A
Savelainen, M
Savini, G
Scott, D
Seiffert, MD
Shellard, EPS
Spencer, LD
Stolyarov, V
Stompor, R
Sudiwala, R
Sutton, D
Suur-Uski, AS
Sygnet, JF
Tauber, JA
Terenzi, L
Toffolatti, L
Tomasi, M
Tristram, M
Tucci, M
Tuovinen, J
Valenziano, L
Valiviita, J
Van Tent, B
Vibert, L
Vielva, P
Villa, F
Wade, LA
Wandelt, BD
Watson, R
Wehus, IK
Yvon, D
Zacchei, A
Zonca, A
AF Adam, R.
Ade, P. A. R.
Aghanim, N.
Arnaud, M.
Ashdown, M.
Aumont, J.
Baccigalupi, C.
Banday, A. J.
Barreiro, R. B.
Bartolo, N.
Battaner, E.
Benabed, K.
Benoit, A.
Benoit-Levy, A.
Bernard, J. -P.
Bersanelli, M.
Bertincourt, B.
Bielewicz, P.
Bock, J. J.
Bonavera, L.
Bond, J. R.
Borrill, J.
Bouchet, F. R.
Boulanger, F.
Bucher, M.
Burigana, C.
Calabrese, E.
Cardoso, J. -F.
Catalano, A.
Challinor, A.
Chamballu, A.
Chiang, H. C.
Christensen, P. R.
Clements, D. L.
Colombi, S.
Colombo, L. P. L.
Combet, C.
Couchot, F.
Coulais, A.
Crill, B. P.
Curto, A.
Cuttaia, F.
Danese, L.
Davies, R. D.
Davis, R. J.
de Bernardis, P.
de Rosa, A.
de Zotti, G.
Delabrouille, J.
Delouis, J. -M.
Desert, F. -X.
Diego, J. M.
Dole, H.
Donzelli, S.
Dore, O.
Douspis, M.
Ducout, A.
Dupac, X.
Efstathiou, G.
Elsner, F.
Ensslin, T. A.
Eriksen, H. K.
Falgarone, E.
Fergusson, J.
Finelli, F.
Forni, O.
Frailis, M.
Fraisse, A. A.
Franceschi, E.
Frejsel, A.
Galeotta, S.
Galli, S.
Ganga, K.
Ghosh, T.
Giard, M.
Giraud-Heraud, Y.
Gjerlow, E.
Gonzalez-Nuevo, J.
Gorski, K. M.
Gratton, S.
Gruppuso, A.
Gudmundsson, J. E.
Hansen, F. K.
Hanson, D.
Harrison, D. L.
Henrot-Versille, S.
Herranz, D.
Hildebrandt, S. R.
Hivon, E.
Hobson, M.
Holmes, W. A.
Hornstrup, A.
Hovest, W.
Huffenberger, K. M.
Hurier, G.
Jaffe, A. H.
Jaffe, T. R.
Jones, W. C.
Juvela, M.
Keihanen, E.
Keskitalo, R.
Kisner, T. S.
Kneissl, R.
Knoche, J.
Kunz, M.
Kurki-Suonio, H.
Lagache, G.
Lamarre, J. -M.
Lasenby, A.
Lattanzi, M.
Lawrence, C. R.
Le Jeune, M.
Leahy, J. P.
Lellouch, E.
Leonardi, R.
Lesgourgues, J.
Levrier, F.
Liguori, M.
Lilje, P. B.
Linden-Vornle, M.
Lopez-Caniego, M.
Lubin, P. M.
Macias-Perez, J. F.
Maggio, G.
Maino, D.
Mandolesi, N.
Mangilli, A.
Maris, M.
Martin, P. G.
Martinez-Gonzalez, E.
Masi, S.
Matarrese, S.
McGehee, P.
Melchiorri, A.
Mendes, L.
Mennella, A.
Migliaccio, M.
Mitra, S.
Miville-Deschenes, M. -A.
Moneti, A.
Montier, L.
Moreno, R.
Morgante, G.
Mortlock, D.
Moss, A.
Mottet, S.
Munshi, D.
Murphy, J. A.
Naselsky, P.
Nati, F.
Natoli, P.
Netterfield, C. B.
Norgaard-Nielsen, H. U.
Noviello, F.
Novikov, D.
Novikov, I.
Oxborrow, C. A.
Paci, F.
Pagano, L.
Pajot, F.
Paoletti, D.
Pasian, F.
Patanchon, G.
Pearson, T. J.
Perdereau, O.
Perotto, L.
Perrotta, F.
Pettorino, V.
Piacentini, F.
Piat, M.
Pierpaoli, E.
Pietrobon, D.
Plaszczynski, S.
Pointecouteau, E.
Polenta, G.
Pratt, G. W.
Prezeau, G.
Prunet, S.
Puget, J. -L.
Rachen, J. P.
Reinecke, M.
Remazeilles, M.
Renault, C.
Renzi, A.
Ristorcelli, I.
Rocha, G.
Rosset, C.
Rossetti, M.
Roudier, G.
Rusholme, B.
Sandri, M.
Santos, D.
Sauve, A.
Savelainen, M.
Savini, G.
Scott, D.
Seiffert, M. D.
Shellard, E. P. S.
Spencer, L. D.
Stolyarov, V.
Stompor, R.
Sudiwala, R.
Sutton, D.
Suur-Uski, A. -S.
Sygnet, J. -F.
Tauber, J. A.
Terenzi, L.
Toffolatti, L.
Tomasi, M.
Tristram, M.
Tucci, M.
Tuovinen, J.
Valenziano, L.
Valiviita, J.
Van Tent, B.
Vibert, L.
Vielva, P.
Villa, F.
Wade, L. A.
Wandelt, B. D.
Watson, R.
Wehus, I. K.
Yvon, D.
Zacchei, A.
Zonca, A.
CA Planck Collaboration
TI Planck 2015 results VIII. High Frequency Instrument data processing:
Calibration and maps
SO ASTRONOMY & ASTROPHYSICS
LA English
DT Article
DE cosmology: observations; cosmic background radiation; surveys; methods:
data analysis
ID PRE-LAUNCH STATUS; MICROWAVE; POLARIZATION; MODEL
AB This paper describes the processing applied to the cleaned, time-ordered information obtained from the Planck High Frequency Instrument (HFI) with the aim of producing photometrically calibrated maps in temperature and (for the first time) in polarization. The data from the entire 2.5-year HFI mission include almost five full-sky surveys. HFI observes the sky over a broad range of frequencies, from 100 to 857 GHz. To obtain the best accuracy on the calibration over such a large range, two different photometric calibration schemes have been used. The 545 and 857 GHz data are calibrated using models of planetary atmospheric emission. The lower frequencies (from 100 to 353 GHz) are calibrated using the time-variable cosmological microwave background dipole, which we call the orbital dipole. This source of calibration only depends on the satellite velocity with respect to the solar system. Using a CMB temperature of T-CMB = 2.7255 +/- 0.0006 K, it permits an independent measurement of the amplitude of the CMB solar dipole (3364.3 +/- 1.5 mu K), which is approximatively 1 sigma higher than the WMAP measurement with a direction that is consistent between the two experiments. We describe the pipeline used to produce the maps of intensity and linear polarization from the HFI timelines, and the scheme used to set the zero level of the maps a posteriori. We also summarize the noise characteristics of the HFI maps in the 2015 Planck data release and present some null tests to assess their quality. Finally, we discuss the major systematic effects and in particular the leakage induced by flux mismatch between the detectors that leads to spurious polarization signal.
C1 [Bucher, M.; Cardoso, J. -F.; Delabrouille, J.; Ganga, K.; Giraud-Heraud, Y.; Le Jeune, M.; Patanchon, G.; Piat, M.; Remazeilles, M.; Rosset, C.; Roudier, G.; Stompor, R.] Univ Paris Diderot, Sorbonne Paris Cite, AstroParticule & Cosmol, APC,CNRS IN2P3,CEA Irfu,Observ Paris, 10 Rue Alice Domon & Leonie Duquet, F-75205 Paris 13, France.
[Kunz, M.] African Inst Math Sci, 6-8 Melrose Rd, ZA-7945 Cape Town, South Africa.
[Natoli, P.; Polenta, G.] Agenzia Spaziale Italiana, Sci Data Ctr, Via Politecn Snc, I-00133 Rome, Italy.
[Lagache, G.] Aix Marseille Univ, CNRS, LAM, UMR 7326, F-13388 Marseille, France.
[Ashdown, M.; Curto, A.; Hobson, M.; Lasenby, A.; Stolyarov, V.] Univ Cambridge, Astrophys Grp, Cavendish Lab, JJ Thomson Ave, Cambridge CB3 0HE, England.
[Chiang, H. C.] Univ KwaZulu Natal, Sch Math Stat & Comp Sci, Astrophys & Cosmol Res Unit, Westville Campus,Private Bag X54001, ZA-4000 Durban, South Africa.
[Kneissl, R.] ALMA Santiago Cent Off, Atacama Large Millimeter submillimeter Array, Alonso Cordova 3107, Santiago 7630355, Chile.
[Bond, J. R.; Hanson, D.; Martin, P. G.; Miville-Deschenes, M. -A.] Univ Toronto, CITA, 60 St George St, Toronto, ON M5S 3H8, Canada.
[Banday, A. J.; Bernard, J. -P.; Bielewicz, P.; Forni, O.; Giard, M.; Jaffe, T. R.; Montier, L.; Pointecouteau, E.; Ristorcelli, I.; Sauve, A.] CNRS, IRAP, 9 Av Colonel Roche,BP 44346, F-31028 Toulouse 4, France.
[Tuovinen, J.] Trinity Coll Dublin, CRANN, Dublin 2, Ireland.
[Bock, J. J.; Crill, B. P.; Dore, O.; Hildebrandt, S. R.; Pearson, T. J.; Prezeau, G.; Rocha, G.; Seiffert, M. D.] CALTECH, Pasadena, CA 91125 USA.
[Challinor, A.; Fergusson, J.; Shellard, E. P. S.] Univ Cambridge, DAMTP, Ctr Theoret Cosmol, Wilberforce Rd, Cambridge CB3 0WA, England.
[Borrill, J.; Keskitalo, R.] Lawrence Berkeley Natl Lab, Computat Cosmol Ctr, Berkeley, CA 92093 USA.
[Chamballu, A.; Yvon, D.] CEA Saclay, DSM Irfu SPP, F-91191 Gif Sur Yvette, France.
[Hornstrup, A.; Linden-Vornle, M.; Norgaard-Nielsen, H. U.; Oxborrow, C. A.] Tech Univ Denmark, DTU Space, Natl Space Inst, Elektrovej 327, DK-2800 Lyngby, Denmark.
[Kunz, M.; Tucci, M.] Univ Geneva, Dept Phys Theor, 24 Quai E Ansermet, CH-1211 Geneva 4, Switzerland.
[Gonzalez-Nuevo, J.; Toffolatti, L.] Univ Oviedo, Dept Fis, Avda Calvo Sotelo S-N, Oviedo 33005, Spain.
[Netterfield, C. B.] Univ Toronto, Dept Astron & Astrophys, 50 St George St, Toronto, ON M5S 3174, Canada.
[Rachen, J. P.] Radboud Univ Nijmegen, Dept Astrophys, IMAPP, POB 9010, NL-6500 GL Nijmegen, Netherlands.
[Scott, D.] Univ British Columbia, Dept Phys & Astron, 6224 Agr Rd, Vancouver, BC V6T 124, Canada.
[Colombo, L. P. L.; Pierpaoli, E.] Univ Southern Calif, Dept Phys & Astron, Dana & David Dornsife Coll Letter Arts & Sci, Los Angeles, CA 90089 USA.
[Elsner, F.] UCL, Dept Phys & Astron, London WC1E 6BT, England.
[Huffenberger, K. M.] Florida State Univ, Dept Phys, Keen Phys Bldg,77 Chieftan Way, Tallahassee, FL 32306 USA.
[Juvela, M.; Keihanen, E.; Kurki-Suonio, H.; Savelainen, M.; Suur-Uski, A. -S.; Valiviita, J.] Univ Helsinki, Dept Phys, Gustaf Hallstromin Katu 2a, Helsinki 00560, Finland.
[Chiang, H. C.; Fraisse, A. A.; Gudmundsson, J. E.; Jones, W. C.; Nati, F.] Princeton Univ, Dept Phys, Princeton, NJ 08540 USA.
[Lubin, P. M.; Zonca, A.] Univ Calif Santa Barbara, Dept Phys, Santa Barbara, CA 93106 USA.
[Wandelt, B. D.] Univ Illinois, Dept Phys, 1110 West Green St, Urbana, IL 61801 USA.
[Bartolo, N.; Liguori, M.; Matarrese, S.] Univ Padua, Dipartimento Fis & Astron G Galilei, Via Marzolo 8, I-35131 Padua, Italy.
[Burigana, C.; Lattanzi, M.; Mandolesi, N.; Natoli, P.] Univ Ferrara, Dipartimento Fis & Sci Terra, Via Saragat 1, I-44122 Ferrara, Italy.
[de Bernardis, P.; Masi, S.; Melchiorri, A.; Pagano, L.; Piacentini, F.] Univ Roma La Sapienza, Dipartimento Fis, Ple A Moro 2, I-00185 Rome, Italy.
[Bersanelli, M.; Maino, D.; Mennella, A.; Rossetti, M.; Tomasi, M.] Univ Milan, Dipartimento Fis, Via Celoria 16, I-20133 Milan, Italy.
[Renzi, A.] Univ Roma Tor Vergata, Dipartimento Matemat, Via Ric Sci 1, I-00133 Rome, Italy.
[Christensen, P. R.; Naselsky, P.] Niels Bohr Inst, Discovery Ctr, Blegdamsvej 17, DK-1165 Copenhagen, Denmark.
[Kneissl, R.] European So Observ, ESO Vitacura, Alonso Cordova 3107, Santiago 19001, Chile.
[Dupac, X.; Leonardi, R.; Lopez-Caniego, M.; Mendes, L.] European Space Agcy, ESAC, Planck Sci Off, Camino Bajo Castillo S-N, Madrid, Spain.
[Tauber, J. A.] European Space Agcy, Estec, Keplerlaan 1, NL-2201 AZ Noordwijk, Netherlands.
[Terenzi, L.] Univ E Campus, Fac Ingn, Via Isimbardi 10, I-22060 Novedrate, CO, Italy.
[Matarrese, S.] INFN, Gran Sasso Sci Inst, I-67100 Laquila, Italy.
[Pettorino, V.] HGSFP, Philosophenweg 16, D-69120 Heidelberg, Germany.
[Pettorino, V.] Heidelberg Univ, Dept Theoret Phys, Philosophenweg 16, D-69120 Heidelberg, Germany.
[Kurki-Suonio, H.; Savelainen, M.; Suur-Uski, A. -S.; Valiviita, J.] Univ Helsinki, Helsinki Inst Phys, Gustaf Hallstromin Katu 2, SF-00100 Helsinki, Finland.
[de Zotti, G.] INAF Osservatorio Astron Padova, Vicolo Osservatorio 5, I-35141 Padua, Italy.
[Polenta, G.] INAF Osservatorio Astron Roma, Via Frascati 33, I-00078 Monte Porzio Catone, Italy.
[Frailis, M.; Galeotta, S.; Maggio, G.; Maris, M.; Pasian, F.; Zacchei, A.] INAF Osservatorio Astron Trieste, Via GB Tiepolo 11, I-34143 Trieste, Italy.
[Burigana, C.; Cuttaia, F.; de Rosa, A.; Finelli, F.; Franceschi, E.; Gruppuso, A.; Mandolesi, N.; Morgante, G.; Natoli, P.; Paoletti, D.; Sandri, M.; Terenzi, L.; Toffolatti, L.; Valenziano, L.; Villa, F.] INAF IASF Bologna, Via Gobetti 101, I-40127 Bologna, Italy.
[Bersanelli, M.; Donzelli, S.; Maino, D.; Mennella, A.; Rossetti, M.; Tomasi, M.] INAF IASF Milano, Via E Bassini 15, Milan 28, Italy.
[Burigana, C.; Finelli, F.; Paoletti, D.] INFN, Sez Bologna, Via Irnerio 46, I-40126 Bologna, Italy.
[Melchiorri, A.; Pagano, L.] Univ Roma Sapienza, INFN, Sez Roma 1, Piazzale Aldo Moro 2, I-00185 Rome, Italy.
[Renzi, A.] Univ Roma Tor Vergata, INFN, Sez Roma 2, Via Ric Sci 1, Rome, Italy.
[Desert, F. -X.] Univ Grenoble Alpes, IPAG, CNRS, F-38000 Grenoble, France.
[Mitra, S.] IUCAA, Post Bag 4,Pune Univ Campus, Pune 411007, Maharashtra, India.
[Clements, D. L.; Ducout, A.; Jaffe, A. H.; Mortlock, D.] Imperial Coll London, Astrophys Grp, Blackett Lab, Prince Consort Rd, London SW7 2AZ, England.
[McGehee, P.; Pearson, T. J.; Rusholme, B.] CALTECH, Infrared Proc & Anal Ctr, Pasadena, CA 91125 USA.
[Benoit, A.] Univ Joseph Fourier Grenoble I, Inst Neel, CNRS, 25 Rue Martyrs, F-38054 Grenoble, France.
[Dole, H.] Inst Univ France, 103 Bd St Michel, F-75005 Paris, France.
[Aghanim, N.; Aumont, J.; Bertincourt, B.; Boulanger, F.; Chamballu, A.; Dole, H.; Douspis, M.; Ghosh, T.; Hurier, G.; Kunz, M.; Lagache, G.; Mangilli, A.; Miville-Deschenes, M. -A.; Pajot, F.; Puget, J. -L.; Remazeilles, M.; Vibert, L.] Univ Paris Sud 11, Inst Astrophys Spatiale, CNRS, UMR 8617, Batiment 121, F-91405 Orsay, France.
[Benabed, K.; Benoit-Levy, A.; Bouchet, F. R.; Cardoso, J. -F.; Colombi, S.; Delouis, J. -M.; Ducout, A.; Elsner, F.; Hivon, E.; Moneti, A.; Mottet, S.; Prunet, S.; Sygnet, J. -F.; Wandelt, B. D.] CNRS, Inst Astrophys Paris, UMR 7095, 98 Bis Blvd Arago, F-75014 Paris, France.
[Lesgourgues, J.] Rhein Westfal TH Aachen, Inst Theoret Teilchenphys & Kosmol, D-52056 Aachen, Germany.
[Challinor, A.; Efstathiou, G.; Gratton, S.; Harrison, D. L.; Migliaccio, M.; Sutton, D.] Univ Cambridge, Inst Astron, Madingley Rd, Cambridge CB3 0HA, England.
[Eriksen, H. K.; Gjerlow, E.; Hansen, F. K.; Lilje, P. B.] Univ Oslo, Inst Theoret Astrophys, N-0371 Oslo, Norway.
[Barreiro, R. B.; Bonavera, L.; Curto, A.; Diego, J. M.; Gonzalez-Nuevo, J.; Herranz, D.; Lopez-Caniego, M.; Martinez-Gonzalez, E.; Toffolatti, L.; Vielva, P.] Univ Cantabria, CSIC, Inst Fis Cantabria, Avda Castros S-N, Santander, Spain.
[Bartolo, N.; Liguori, M.; Matarrese, S.] Ist Nazl Fis Nucl, Sez Padova, Via Marzolo 8, I-35131 Padua, Italy.
[Bock, J. J.; Colombo, L. P. L.; Crill, B. P.; Dore, O.; Gorski, K. M.; Hanson, D.; Hildebrandt, S. R.; Holmes, W. A.; Lawrence, C. R.; Mitra, S.; Pietrobon, D.; Prezeau, G.; Rocha, G.; Roudier, G.; Seiffert, M. D.; Wade, L. A.; Wehus, I. K.] CALTECH, Jet Prop Lab, 4800 Oak Grove Dr, Pasadena, CA 91109 USA.
[Davies, R. D.; Davis, R. J.; Leahy, J. P.; Noviello, F.; Remazeilles, M.; Watson, R.] Univ Manchester, Sch Phys & Astron, Jodrell Bank Ctr Astrophys, Alan Turing Bldg,Oxford Rd, Manchester M13 9PL, Lancs, England.
[Galli, S.] Univ Chicago, Kavli Inst Cosmol Phys, Chicago, IL 60637 USA.
[Ashdown, M.; Challinor, A.; Curto, A.; Gratton, S.; Harrison, D. L.; Lasenby, A.; Migliaccio, M.; Sutton, D.] Kavli Inst Cosmol Cambridge, Madingley Rd, Cambridge CB3 0HA, England.
[Stolyarov, V.] Kazan Fed Univ, 18 Kremlyovskaya St, Kazan 420008, Russia.
[Couchot, F.; Henrot-Versille, S.; Mangilli, A.; Perdereau, O.; Plaszczynski, S.; Tristram, M.] Univ Paris 11, LAL, CNRS, IN2P3, Orsay, France.
[Catalano, A.; Coulais, A.; Falgarone, E.; Lamarre, J. -M.; Levrier, F.; Roudier, G.] Observ Paris, CNRS, LERMA, 61 Ave Observ, F-75014 Paris, France.
[Lellouch, E.; Moreno, R.] Univ Paris Diderot, UPMC, CNRS, Observ Paris,LESIA, 5 Pl J Janssen, F-92195 Meudon, France.
[Arnaud, M.; Chamballu, A.; Pratt, G. W.] Univ Paris Diderot, CNRS, Lab AIM, IRFU,Serv Astrophys,CEA DSM,CEA Saclay, Bat 709, F-91191 Gif Sur Yvette, France.
[Cardoso, J. -F.] CNRS, Lab Traitement & Commun Informat, UMR 5141, 46 Rue Barrault, F-75634 Paris 13, France.
[Cardoso, J. -F.] Telecom ParisTech, 46 Rue Barrault, F-75634 Paris 13, France.
[Adam, R.; Catalano, A.; Combet, C.; Macias-Perez, J. F.; Perotto, L.; Renault, C.; Santos, D.] Univ Grenoble Alpes, Lab Phys Subatom & Cosmol, CNRS, IN2P3, 53 Rue Martyrs, F-38026 Grenoble, France.
[Van Tent, B.] Univ Paris Sud 11, Phys Theor Lab, Batiment 210, F-91405 Orsay, France.
[Van Tent, B.] CNRS, Batiment 210, F-91405 Orsay, France.
[Kisner, T. S.] Lawrence Berkeley Natl Lab, Berkeley, CA 94720 USA.
[Novikov, D.; Novikov, I.] Russian Acad Sci, Ctr Astro Space, Lebedev Phys Inst, 84-32 Profsoyuznaya St,GSP 7, Moscow 117997, Russia.
[Ensslin, T. A.; Hovest, W.; Knoche, J.; Rachen, J. P.; Reinecke, M.] Max Planck Inst Astrophys, Karl Schwarzschild Str 1, D-85741 Garching, Germany.
[Hanson, D.] McGill Univ, McGill Phys, Ernest Rutherford Phys Bldg,3600 Rue Univ, Montreal, PQ H3A 2T8, Canada.
[Murphy, J. A.] Natl Univ Ireland, Dept Expt Phys, Maynooth, Kildare, Ireland.
[Bielewicz, P.] Nicolaus Copernicus Astron Ctr, Bartycka 18, PL-00716 Warsaw, Poland.
[Christensen, P. R.; Frejsel, A.; Naselsky, P.; Novikov, I.] Niels Bohr Inst, Blegdamsvej 17, DK-2100 Copenhagen, Denmark.
[Savini, G.] UCL, Opt Sci Lab, Gower St, London WC1E 6BT, England.
[Baccigalupi, C.; Bielewicz, P.; Danese, L.; de Zotti, G.; Paci, F.; Perrotta, F.] SISSA, Astrophys Sect, Via Bonomea 265, I-34136 Trieste, Italy.
[Ade, P. A. R.; Munshi, D.; Spencer, L. D.; Sudiwala, R.] Cardiff Univ, Sch Phys & Astron, Queens Bldg, Cardiff CF24 3AA, S Glam, Wales.
[Moss, A.] Univ Nottingham, Sch Phys & Astron, Nottingham NG7 2RD, England.
[Bouchet, F. R.] Sorbonne Univ, UPMC, UMR 7095, Inst Astrophys Paris, 98 Bis Blvd Arago, F-75014 Paris, France.
[Borrill, J.] Univ Calif Berkeley, Space Sci Lab, Berkeley, CA 94720 USA.
[Stolyarov, V.] Russian Acad Sci, Special Astrophys Observ, Nizhnii Arkhyz 369167, Zelenchukskiy R, Russia.
[Calabrese, E.] Univ Oxford, Subdept Astrophys, Keble Rd, Oxford OX1 3RH, England.
[Lesgourgues, J.] CERN, Div Theory, PH TH, CH-1211 Geneva 23, Switzerland.
[Benabed, K.; Benoit-Levy, A.; Colombi, S.; Delouis, J. -M.; Elsner, F.; Hivon, E.; Prunet, S.; Wandelt, B. D.] Univ Paris 06, UPMC, UMR 7095, 98 Bis Blvd Arago, F-75014 Paris, France.
[Banday, A. J.; Bernard, J. -P.; Forni, O.; Giard, M.; Jaffe, T. R.; Montier, L.; Pointecouteau, E.; Ristorcelli, I.; Sauve, A.] Univ Toulouse, UPS OMP, IRAP, F-31028 Toulouse 4, France.
[Battaner, E.] Univ Granada, Dept Fis Teor & Cosmos, Fac Ciencias, Granada 18001, Spain.
[Battaner, E.] Univ Granada, Inst Carlos Fis Teor & Computac 1, Granada 18003, Spain.
[Gorski, K. M.] Univ Warsaw Observ, Aleje Ujazdowskie 4, PL-00478 Warsaw, Poland.
RP Perdereau, O; Tristram, M (reprint author), Univ Paris 11, LAL, CNRS, IN2P3, Orsay, France.
EM perdereau@lal.in2p3.fr; tristram@lal.in2p3.fr
RI Barreiro, Rita Belen/N-5442-2014; bonavera, laura/E-9368-2017;
Gonzalez-Nuevo, Joaquin/I-3562-2014; Herranz, Diego/K-9143-2014;
Colombo, Loris/J-2415-2016;
OI Barreiro, Rita Belen/0000-0002-6139-4272; Valiviita,
Jussi/0000-0001-6225-3693; Hurier, Guillaume/0000-0002-1215-0706; Hivon,
Eric/0000-0003-1880-2733; bonavera, laura/0000-0001-8039-3876;
Gonzalez-Nuevo, Joaquin/0000-0003-1354-6822; Herranz,
Diego/0000-0003-4540-1417; Colombo, Loris/0000-0003-4572-7732; Zacchei,
Andrea/0000-0003-0396-1192; Stolyarov, Vladislav/0000-0001-8151-828X;
TERENZI, LUCA/0000-0001-9915-6379; Toffolatti,
Luigi/0000-0003-2645-7386; Lilje, Per/0000-0003-4324-7794; Paoletti,
Daniela/0000-0003-4761-6147; Nati, Federico/0000-0002-8307-5088; Savini,
Giorgio/0000-0003-4449-9416; Pierpaoli, Elena/0000-0002-7957-8993
FU ESA; CNES (France); CNRS/INSU-IN2P3-INP (France); ASI (Italy); CNR
(Italy); INAF (Italy); NASA (USA); DoE (USA); STFC (UK); UKSA (UK); CSIC
(Spain); MINECO (Spain); JA (Spain); RES (Spain); Tekes (Finland); AoF
(Finland); CSC (Finland); DLR (Germany); MPG (Germany); CSA (Canada);
DTU Space (Denmark); SER/SSO (Switzerland); RCN (Norway); SFI (Ireland);
FCT/MCTES (Portugal); ERC (EU); PRACE (EU)
FX The Planck Collaboration acknowledges the support of: ESA; CNES and
CNRS/INSU-IN2P3-INP (France); ASI, CNR, and INAF (Italy); NASA and DoE
(USA); STFC and UKSA (UK); CSIC, MINECO, JA, and RES (Spain); Tekes,
AoF, and CSC (Finland); DLR and MPG (Germany); CSA (Canada); DTU Space
(Denmark); SER/SSO (Switzerland); RCN (Norway); SFI (Ireland); FCT/MCTES
(Portugal); ERC and PRACE (EU). A description of the Planck
Collaboration and a list of its members, indicating which technical or
scientific activities they have been involved in, can be found at
http://www.cosmos.esa.int/web/planck/planck-collaboration.
NR 52
TC 3
Z9 3
U1 1
U2 1
PU EDP SCIENCES S A
PI LES ULIS CEDEX A
PA 17, AVE DU HOGGAR, PA COURTABOEUF, BP 112, F-91944 LES ULIS CEDEX A,
FRANCE
SN 1432-0746
J9 ASTRON ASTROPHYS
JI Astron. Astrophys.
PD OCT
PY 2016
VL 594
AR A8
DI 10.1051/0004-6361/201525820
PG 27
WC Astronomy & Astrophysics
SC Astronomy & Astrophysics
GA DZ4MG
UT WOS:000385832200008
ER
PT J
AU Adam, R
Ade, PAR
Aghanim, N
Alves, MIR
Arnaud, M
Ashdown, M
Aumont, J
Baccigalupi, C
Banday, AJ
Barreiro, RB
Bartlett, JG
Bartolo, N
Battaner, E
Benabed, K
Benoit, A
Benoit-Levy, A
Bernard, JP
Bersanelli, M
Bielewicz, P
Bock, JJ
Bonaldi, A
Bonavera, L
Bond, JR
Borrill, J
Bouchet, FR
Boulanger, F
Bucher, M
Burigana, C
Butler, RC
Calabrese, E
Cardoso, JF
Catalano, A
Challinor, A
Chamballu, A
Chary, RR
Chiang, HC
Christensen, PR
Clements, DL
Colombi, S
Colombo, LPL
Combet, C
Couchot, F
Coulais, A
Crill, BP
Curto, A
Cuttaia, F
Danese, L
Davies, RD
Davis, RJ
de Bernardis, P
de Rosa, A
de Zotti, G
Delabrouille, J
Desert, FX
Dickinson, C
Diego, JM
Dole, H
Donzelli, S
Dore, O
Douspis, M
Ducout, A
Dupac, X
Efstathiou, G
Elsner, F
Ensslin, TA
Eriksen, HK
Falgarone, E
Fergusson, J
Finelli, F
Forni, O
Frailis, M
Fraisse, AA
Franceschi, E
Frejsel, A
Galeotta, S
Galli, S
Ganga, K
Ghosh, T
Giard, M
Giraud-Heraud, Y
Gjerlow, E
Gonzalez-Nuevo, J
Gorski, KM
Gratton, S
Gregorio, A
Gruppuso, A
Gudmundsson, JE
Hansen, FK
Hanson, D
Harrison, DL
Helou, G
Henrot-Versille, S
Hernandez-Monteagudo, C
Herranz, D
Hildebrandt, SR
Hivon, F
Hobson, M
Holmes, WA
Hornstrup, A
Hovest, W
Huffenberger, KM
Hurier, G
Jaffe, AH
Jaffe, TR
Jones, WC
Juvela, M
Keihaen, E
Keskitalo, R
Kisner, TS
Kneissl, R
Knoche, J
Kunz, M
Kurki-Suonio, H
Lagache, G
Lahteenmaki, A
Lamarre, JM
Lasenby, A
Lattanzi, M
Lawrence, CR
Le Jeune, M
Leahy, JP
Leonardi, R
Lesgourgues, J
Levrier, F
Liguori, M
Lilje, PB
Linden-Vornle, M
Lopez-Caniego, M
Lubin, PM
Macias-Perez, JF
Maggio, G
Maino, D
Mandolesi, N
Mangilli, A
Maris, M
Marshall, DJ
Martin, PG
Martinez-Gonzalez, E
Masi, S
Matarrese, S
McGehee, P
Meinhold, PR
Melchiorri, A
Mendes, L
Mennella, A
Migliaccio, M
Mitra, S
Miville-Deschenes, MA
Moneti, A
Montier, L
Morgante, G
Mortlock, D
Moss, A
Munshi, D
Murphy, JA
Naselsky, P
Nati, F
Natoli, P
Netterfield, CB
Norgaard-Nielsen, HU
Noviello, F
Novikov, D
Novikov, I
Orlando, E
Oxborrow, CA
Paci, F
Pagano, L
Pajot, F
Paladini, R
Paoletti, D
Partridge, B
Pasian, F
Patanchon, G
Pearson, TJ
Perdereau, O
Perotto, L
Perrotta, F
Pettorino, V
Piacentini, F
Piat, M
Pierpaoli, E
Pietrobon, D
Plaszczynski, S
Pointecouteau, E
Polenta, G
Pratt, GW
Prezeau, G
Prunet, S
Puget, JL
Rachen, JP
Reach, WT
Rebolo, R
Reinecke, M
Remazeilles, M
Renault, C
Renzi, A
Ristorcelli, I
Rocha, G
Rosset, C
Rossetti, M
Roudier, G
Rubino-Martin, JA
Rusholme, B
Sandri, M
Santos, D
Savelainen, M
Savini, G
Scott, D
Seiffert, MD
Shellard, EPS
Spencer, LD
Stolyarov, V
Stompor, R
Strong, AW
Sudiwala, R
Sunyaev, R
Sutton, D
Suur-Uski, AS
Sygnet, JF
Tauber, JA
Terenzi, L
Toffolatti, L
Tomasi, M
Tristram, M
Tucci, M
Tuovinen, J
Umana, G
Valenziano, L
Valiviita, J
Van Tent, F
Vielva, P
Villa, F
Wade, LA
Wandelt, BD
Wehus, IK
Wilkinson, A
Yvon, D
Zacchei, A
Zonca, A
AF Adam, R.
Ade, P. A. R.
Aghanim, N.
Alves, M. I. R.
Arnaud, M.
Ashdown, M.
Aumont, J.
Baccigalupi, C.
Banday, A. J.
Barreiro, R. B.
Bartlett, J. G.
Bartolo, N.
Battaner, E.
Benabed, K.
Benoit, A.
Benoit-Levy, A.
Bernard, J. -P.
Bersanelli, M.
Bielewicz, P.
Bock, J. J.
Bonaldi, A.
Bonavera, L.
Bond, J. R.
Borrill, J.
Bouchet, F. R.
Boulanger, F.
Bucher, M.
Burigana, C.
Butler, R. C.
Calabrese, E.
Cardoso, J. -F.
Catalano, A.
Challinor, A.
Chamballu, A.
Chary, R. -R.
Chiang, H. C.
Christensen, P. R.
Clements, D. L.
Colombi, S.
Colombo, L. P. L.
Combet, C.
Couchot, F.
Coulais, A.
Crill, B. P.
Curto, A.
Cuttaia, F.
Danese, L.
Davies, R. D.
Davis, R. J.
de Bernardis, P.
de Rosa, A.
de Zotti, G.
Delabrouille, J.
Desert, F. -X.
Dickinson, C.
Diego, J. M.
Dole, H.
Donzelli, S.
Dore, O.
Douspis, M.
Ducout, A.
Dupac, X.
Efstathiou, G.
Elsner, F.
Ensslin, T. A.
Eriksen, H. K.
Falgarone, E.
Fergusson, J.
Finelli, F.
Forni, O.
Frailis, M.
Fraisse, A. A.
Franceschi, E.
Frejsel, A.
Galeotta, S.
Galli, S.
Ganga, K.
Ghosh, T.
Giard, M.
Giraud-Heraud, Y.
Gjerlow, E.
Gonzalez-Nuevo, J.
Gorski, K. M.
Gratton, S.
Gregorio, A.
Gruppuso, A.
Gudmundsson, J. E.
Hansen, F. K.
Hanson, D.
Harrison, D. L.
Helou, G.
Henrot-Versille, S.
Hernandez-Monteagudo, C.
Herranz, D.
Hildebrandt, S. R.
Hivon, F.
Hobson, M.
Holmes, W. A.
Hornstrup, A.
Hovest, W.
Huffenberger, K. M.
Hurier, G.
Jaffe, A. H.
Jaffe, T. R.
Jones, W. C.
Juvela, M.
Keihanen, E.
Keskitalo, R.
Kisner, T. S.
Kneissl, R.
Knoche, J.
Kunz, M.
Kurki-Suonio, H.
Lagache, G.
Lahteenmaki, A.
Lamarre, J. -M.
Lasenby, A.
Lattanzi, M.
Lawrence, C. R.
Le Jeune, M.
Leahy, J. P.
Leonardi, R.
Lesgourgues, J.
Levrier, F.
Liguori, M.
Lilje, P. B.
Linden-Vornle, M.
Lopez-Caniego, M.
Lubin, P. M.
Macias-Perez, J. F.
Maggio, G.
Maino, D.
Mandolesi, N.
Mangilli, A.
Maris, M.
Marshall, D. J.
Martin, P. G.
Martinez-Gonzalez, E.
Masi, S.
Matarrese, S.
McGehee, P.
Meinhold, P. R.
Melchiorri, A.
Mendes, L.
Mennella, A.
Migliaccio, M.
Mitra, S.
Miville-Deschenes, M. -A.
Moneti, A.
Montier, L.
Morgante, G.
Mortlock, D.
Moss, A.
Munshi, D.
Murphy, J. A.
Naselsky, P.
Nati, F.
Natoli, P.
Netterfield, C. B.
Norgaard-Nielsen, H. U.
Noviello, F.
Novikov, D.
Novikov, I.
Orlando, E.
Oxborrow, C. A.
Paci, F.
Pagano, L.
Pajot, F.
Paladini, R.
Paoletti, D.
Partridge, B.
Pasian, F.
Patanchon, G.
Pearson, T. J.
Perdereau, O.
Perotto, L.
Perrotta, F.
Pettorino, V.
Piacentini, F.
Piat, M.
Pierpaoli, E.
Pietrobon, D.
Plaszczynski, S.
Pointecouteau, E.
Polenta, G.
Pratt, G. W.
Prezeau, G.
Prunet, S.
Puget, J. -L.
Rachen, J. P.
Reach, W. T.
Rebolo, R.
Reinecke, M.
Remazeilles, M.
Renault, C.
Renzi, A.
Ristorcelli, I.
Rocha, G.
Rosset, C.
Rossetti, M.
Roudier, G.
Rubino-Martin, J. A.
Rusholme, B.
Sandri, M.
Santos, D.
Savelainen, M.
Savini, G.
Scott, D.
Seiffert, M. D.
Shellard, E. P. S.
Spencer, L. D.
Stolyarov, V.
Stompor, R.
Strong, A. W.
Sudiwala, R.
Sunyaev, R.
Sutton, D.
Suur-Uski, A. -S.
Sygnet, J. -F.
Tauber, J. A.
Terenzi, L.
Toffolatti, L.
Tomasi, M.
Tristram, M.
Tucci, M.
Tuovinen, J.
Umana, G.
Valenziano, L.
Valiviita, J.
Van Tent, F.
Vielva, P.
Villa, F.
Wade, L. A.
Wandelt, B. D.
Wehus, I. K.
Wilkinson, A.
Yvon, D.
Zacchei, A.
Zonca, A.
CA Planck Collaboration
TI Planck 2015 results X. Diffuse component separation: Foreground maps
SO ASTRONOMY & ASTROPHYSICS
LA English
DT Article
DE ISM: general; cosmology: observations; polarization; cosmic background
radiation; diffuse radiation; Galaxy: general
ID MICROWAVE-ANISOTROPY-PROBE; POWER SPECTRUM ESTIMATION; COSMIC-RAY
PROPAGATION; LATITUDE MOLECULAR GAS; WMAP OBSERVATIONS; GALACTIC PLANE;
BACKGROUND-RADIATION; DUST EMISSION; DATA RELEASE; MILKY-WAY
AB Planck has mapped the microwave sky in temperature over nine frequency bands between 30 and 857 GHz and in polarization over seven frequency bands between 30 and 353 GHz in polarization. In this paper we consider the problem of diffuse astrophysical component separation, and process these maps within a Bayesian framework to derive an internally consistent set of full-sky astrophysical component maps. Component separation dedicated to cosmic microwave background (CMB) reconstruction is described in a companion paper. For the temperature analysis, we combine the Planck observations with the 9-yr Wilkinson Microwave Anisotropy Probe (WMAP) sky maps and the Haslam et al. 408 MHz map, to derive a joint model of CMB, synchrotron, free-free, spinning dust, CO, line emission in the 94 and 100 GHz channels, and thermal dust emission. Full-sky maps are provided for each component, with an angular resolution varying between 7: 5 and 1 degrees. Global parameters (monopoles, dipoles, relative calibration, and bandpass errors) are fitted jointly with the sky model, and best-fit values are tabulated. For polarization, the model includes CMB, synchrotron, and thermal dust emission. These models provide excellent fits to the observed data, with rms temperature residuals smaller than 4pK over 93% of the sky for all Planck frequencies up to 353 GHz, and fractional errors smaller than 1% in the remaining 7% of the sky. The main limitations of the temperature model at the lower frequencies are internal degeneracies among the spinning dust, free-free, and synchrotron components; additional observations from external low-frequency experiments will be essential to break these degeneracies. The main limitations of the temperature model at the higher frequencies are uncertainties in the 545 and 857 GHz calibration and zero-points. For polarization, the main outstanding issues are instrumental systematics in the 100-353 GHz bands on large angular scales in the form of temperature-to-polarization leakage, uncertainties in the analogue-to-digital conversion, and corrections for the very long time constant of the bolometer detectors, all of which are expected to improve in the near future.
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[Natoli, P.; Polenta, G.] Agenzia Spaziale Italiana Sci Data Ctr, Via Politecn Snc, I-00133 Rome, Italy.
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[Alves, M. I. R.; Banday, A. J.; Bernard, J. -P.; Forni, O.; Giard, M.; Jaffe, T. R.; Montier, L.; Pointecouteau, E.; Ristorcelli, I.] Univ Toulouse, UPS OMP, TRAP, F-31028 Toulouse 4, France.
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RP Wehus, IK (reprint author), Inst Astrofis Canarias, C Via Lactea S-N, Tenerife 38205, Spain.; Wehus, IK (reprint author), CALTECH, Jet Prop Lab, 4800 Oak Grove Dr, Pasadena, CA 31109 USA.
EM i.k.wehus@astro.uio.no
RI Lahteenmaki, Anne/L-5987-2013; Barreiro, Rita Belen/N-5442-2014;
bonavera, laura/E-9368-2017; Gonzalez-Nuevo, Joaquin/I-3562-2014;
Herranz, Diego/K-9143-2014; Colombo, Loris/J-2415-2016;
OI Valiviita, Jussi/0000-0001-6225-3693; Toffolatti,
Luigi/0000-0003-2645-7386; Lilje, Per/0000-0003-4324-7794; Nati,
Federico/0000-0002-8307-5088; Savini, Giorgio/0000-0003-4449-9416;
Pierpaoli, Elena/0000-0002-7957-8993; Paoletti,
Daniela/0000-0003-4761-6147; TERENZI, LUCA/0000-0001-9915-6379;
Barreiro, Rita Belen/0000-0002-6139-4272; bonavera,
laura/0000-0001-8039-3876; Reach, William/0000-0001-8362-4094;
Gonzalez-Nuevo, Joaquin/0000-0003-1354-6822; Herranz,
Diego/0000-0003-4540-1417; Colombo, Loris/0000-0003-4572-7732; Zacchei,
Andrea/0000-0003-0396-1192; Stolyarov, Vladislav/0000-0001-8151-828X
FU ESA; CNES (France); CNRS/INSU-IN2P3-INP (France); ASI (Italy); CNR
(Italy); INAF (Italy); NASA (USA); DoE (USA); STFC (UK); UKSA (UK); CSIC
(Spain); MINECO (Spain); JA (Spain); RES (Spain); Tekes (Finland); AoF
(Finland); CSC (Finland); DLR (Germany); MPG (Germany); CSA (Canada);
DTU Space (Denmark); SER/SSO (Switzerland); RCN (Norway); SFI (Ireland);
FCT/MCTES (Portugal); ERC (EU); PRACE (EU)
FX The Planck Collaboration acknowledges the support of: ESA; CNES, and
CNRS/INSU-IN2P3-INP (France); ASI, CNR, and INAF (Italy); NASA and DoE
(USA); STFC and UKSA (UK); CSIC, MINECO, JA and RES (Spain); Tekes, AoF,
and CSC (Finland); DLR and MPG (Germany); CSA (Canada); DTU Space
(Denmark); SER/SSO (Switzerland); RCN (Norway); SFI (Ireland); FCT/MCTES
(Portugal); ERC and PRACE (EU). A description of the Planck
Collaboration and a list of its members, indicating which technical or
scientific activities they have been involved in, can be found at
http://www.cosmos.esa.int/web/planck/planck-collaboration.
NR 126
TC 3
Z9 3
U1 0
U2 0
PU EDP SCIENCES S A
PI LES ULIS CEDEX A
PA 17, AVE DU HOGGAR, PA COURTABOEUF, BP 112, F-91944 LES ULIS CEDEX A,
FRANCE
SN 1432-0746
J9 ASTRON ASTROPHYS
JI Astron. Astrophys.
PD OCT
PY 2016
VL 594
AR A10
DI 10.1051/0004-6361/201525967
PG 63
WC Astronomy & Astrophysics
SC Astronomy & Astrophysics
GA DZ4MG
UT WOS:000385832200021
ER
PT J
AU Adam, R
Ade, PAR
Aghanim, N
Arnaud, M
Ashdown, M
Aumont, J
Baccigalupi, C
Banday, AJ
Barreiro, RB
Bartlett, JG
Bartolo, N
Basak, S
Battaner, E
Benabed, K
Benoit, A
Benoit-Levy, A
Bernard, JP
Bersanelli, M
Bielewicz, P
Bock, JJ
Bonaldi, A
Bonavera, L
Bond, JR
Borrill, J
Bouchet, FR
Boulanger, F
Bucher, M
Burigana, C
Butler, RC
Calabrese, E
Cardoso, JF
Casaponsa, B
Castex, G
Catalano, A
Challinor, A
Chamballu, A
Chary, RR
Chiang, HC
Christensen, PR
Clements, DL
Colombi, S
Colombo, LPL
Combet, C
Couchot, F
Coulais, A
Crill, BP
Curto, A
Cuttaia, F
Danese, L
Davies, RD
Davis, RJ
de Bernardis, P
de Rosa, A
de Zotti, G
Delabrouille, J
Desert, FX
Dickinson, C
Diego, JM
Dole, H
Donzelli, S
Dore, O
Douspis, M
Ducout, A
Dupac, X
Efstathiou, G
Elsner, F
Ensslin, TA
Eriksen, HK
Falgarone, E
Fantaye, Y
Fergusson, J
Finelli, F
Forni, O
Frailis, M
Fraisse, AA
Francescht, E
Frejsel, A
Galeotta, S
Galli, S
Ganga, K
Ghosh, T
Giard, M
Giraud-Heraud, Y
Gjerlow, E
Gonzalez-Nuevo, J
Gorski, KM
Gratton, S
Gregorio, A
Gruppuso, A
Gudmundsson, JE
Hansen, FK
Hanson, D
Harrison, DL
Helou, G
Henrot-Versille, S
Hernandez-Monteagudo, C
Herranz, D
Hildebrandt, SR
Hivon, E
Hobson, M
Holmes, WA
Hornstrup, A
Hovest, W
Huffenberger, KM
Hurier, G
Jaffe, AH
Jaffe, TR
Jones, WC
Juvela, M
Keihanen, E
Keskitalo, R
Kisner, TS
Kneissl, R
Knoche, J
Krachmalnicoff, N
Kunz, M
Kurki-Suonio, H
Lagache, G
Lamarre, JM
Lasenby, A
Lattanzi, M
Lawrence, CR
Le Jenne, M
Leonardi, R
Lesgourgues, J
Levrier, F
Liguori, M
Lilje, PB
Linden-Vornle, M
Lopez-Caniego, M
Lubin, PM
Macias-Perez, JF
Maggio, G
Maino, D
Mandolesi, N
Mangilli, A
Maris, M
Marshall, DJ
Martin, PG
Martinez-Gonzalez, E
Masi, S
Matarrese, S
McGehee, P
Meinhold, PR
Melchiorri, A
Mendes, L
Mennella, A
Migliaccio, M
Mitra, S
Miville-Deschenes, MA
Molinari, D
Moneti, A
Montier, L
Morgante, G
Mortlock, D
Moss, A
Munshi, D
Murphy, JA
Naselsky, P
Nati, F
Natoli, P
Netterfield, CB
Norgaard-Nielsen, HU
Noviello, F
Novikov, D
Novikov, I
Oxborrow, CA
Paci, F
Pagano, L
Pajot, F
Paladini, R
Paoletti, D
Pasian, F
Patanchon, G
Pearson, TJ
Perdereau, O
Perotto, L
Perrotta, F
Pettorino, V
Piacentini, F
Piat, M
Pierpaoli, E
Pietrobon, D
Plaszczynski, S
Pointecouteau, E
Polenta, G
Pratt, GW
Prezeau, G
Prunet, S
Puget, JL
Rachen, JP
Racine, B
Reach, WT
Rebolo, R
Reinecke, M
Remazeilles, M
Renault, C
Renzi, A
Ristorcelli, I
Rocha, G
Rosset, C
Rossetti, M
Roudier, G
Rubino-Martin, JA
Rusholme, B
Sandri, M
Santos, D
Savelainen, M
Savini, G
Scott, D
Seiffert, MD
Shellard, EPS
Spencer, LD
Stolyarov, V
Stompor, R
Sudiwala, R
Sunyaev, R
Sutton, D
Suur-Uski, AS
Sygnet, JF
Tauber, JA
Terenzi, L
Toffolatti, L
Tomasi, M
Tristram, M
Trombetti, T
Tucci, M
Tuovinen, J
Valenziano, L
Valiviita, J
Van Tent, F
Vielva, P
Villa, F
Wade, LA
Wandelt, BD
Wehus, IK
Yvon, D
Zacchei, A
Zonca, A
AF Adam, R.
Ade, P. A. R.
Aghanim, N.
Arnaud, M.
Ashdown, M.
Aumont, J.
Baccigalupi, C.
Banday, A. J.
Barreiro, R. B.
Bartlett, J. G.
Bartolo, N.
Basak, S.
Battaner, E.
Benabed, K.
Benoit, A.
Benoit-Levy, A.
Bernard, J. -P.
Bersanelli, M.
Bielewicz, P.
Bock, J. J.
Bonaldi, A.
Bonavera, L.
Bond, J. R.
Borrill, J.
Bouchet, F. R.
Boulanger, F.
Bucher, M.
Burigana, C.
Butler, R. C.
Calabrese, E.
Cardoso, J. -F.
Casaponsa, B.
Castex, G.
Catalano, A.
Challinor, A.
Chamballu, A.
Chary, R-R.
Chiang, H. C.
Christensen, P. R.
Clements, D. L.
Colombi, S.
Colombo, L. P. L.
Combet, C.
Couchot, F.
Coulais, A.
Crill, B. P.
Curto, A.
Cuttaia, F.
Danese, L.
Davies, R. D.
Davis, R. J.
de Bernardis, P.
de Rosa, A.
de Zotti, G.
Delabrouille, J.
Desert, F. -X.
Dickinson, C.
Diego, J. M.
Dole, H.
Donzelli, S.
Dore, O.
Douspis, M.
Ducout, A.
Dupac, X.
Efstathiou, G.
Elsner, F.
Ensslin, T. A.
Eriksen, H. K.
Falgarone, E.
Fantaye, Y.
Fergusson, J.
Finelli, F.
Forni, O.
Frailis, M.
Fraisse, A. A.
Francescht, E.
Frejsel, A.
Galeotta, S.
Galli, S.
Ganga, K.
Ghosh, T.
Giard, M.
Giraud-Heraud, Y.
Gjerlow, E.
Gonzalez-Nuevo, J.
Gorski, K. M.
Gratton, S.
Gregorio, A.
Gruppuso, A.
Gudmundsson, J. E.
Hansen, F. K.
Hanson, D.
Harrison, D. L.
Helou, G.
Henrot-Versille, S.
Hernandez-Monteagudo, C.
Herranz, D.
Hildebrandt, S. R.
Hivon, E.
Hobson, M.
Holmes, W. A.
Hornstrup, A.
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Huffenberger, K. M.
Hurier, G.
Jaffe, A. H.
Jaffe, T. R.
Jones, W. C.
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Keihanen, E.
Keskitalo, R.
Kisner, T. S.
Kneissl, R.
Knoche, J.
Krachmalnicoff, N.
Kunz, M.
Kurki-Suonio, H.
Lagache, G.
Lamarre, J. -M.
Lasenby, A.
Lattanzi, M.
Lawrence, C. R.
Le Jenne, M.
Leonardi, R.
Lesgourgues, J.
Levrier, F.
Liguori, M.
Lilje, P. B.
Linden-Vornle, M.
Lopez-Caniego, M.
Lubin, P. M.
Macias-Perez, J. F.
Maggio, G.
Maino, D.
Mandolesi, N.
Mangilli, A.
Maris, M.
Marshall, D. J.
Martin, P. G.
Martinez-Gonzalez, E.
Masi, S.
Matarrese, S.
McGehee, P.
Meinhold, P. R.
Melchiorri, A.
Mendes, L.
Mennella, A.
Migliaccio, M.
Mitra, S.
Miville-Deschenes, M. -A.
Molinari, D.
Moneti, A.
Montier, L.
Morgante, G.
Mortlock, D.
Moss, A.
Munshi, D.
Murphy, J. A.
Naselsky, P.
Nati, F.
Natoli, P.
Netterfield, C. B.
Norgaard-Nielsen, H. U.
Noviello, F.
Novikov, D.
Novikov, I.
Oxborrow, C. A.
Paci, F.
Pagano, L.
Pajot, F.
Paladini, R.
Paoletti, D.
Pasian, F.
Patanchon, G.
Pearson, T. J.
Perdereau, O.
Perotto, L.
Perrotta, F.
Pettorino, V.
Piacentini, F.
Piat, M.
Pierpaoli, E.
Pietrobon, D.
Plaszczynski, S.
Pointecouteau, E.
Polenta, G.
Pratt, G. W.
Prezeau, G.
Prunet, S.
Puget, J. -L.
Rachen, J. P.
Racine, B.
Reach, W. T.
Rebolo, R.
Reinecke, M.
Remazeilles, M.
Renault, C.
Renzi, A.
Ristorcelli, I.
Rocha, G.
Rosset, C.
Rossetti, M.
Roudier, G.
Rubino-Martin, J. A.
Rusholme, B.
Sandri, M.
Santos, D.
Savelainen, M.
Savini, G.
Scott, D.
Seiffert, M. D.
Shellard, E. P. S.
Spencer, L. D.
Stolyarov, V.
Stompor, R.
Sudiwala, R.
Sunyaev, R.
Sutton, D.
Suur-Uski, A. -S.
Sygnet, J. -F.
Tauber, J. A.
Terenzi, L.
Toffolatti, L.
Tomasi, M.
Tristram, M.
Trombetti, T.
Tucci, M.
Tuovinen, J.
Valenziano, L.
Valiviita, J.
Van Tent, F.
Vielva, P.
Villa, F.
Wade, L. A.
Wandelt, B. D.
Wehus, I. K.
Yvon, D.
Zacchei, A.
Zonca, A.
CA Planck Collaboration
TI Planck 2015 results IX. Diffuse component separation: CMB maps
SO ASTRONOMY & ASTROPHYSICS
LA English
DT Article
DE cosmology: observations; polarization; cosmic background radiation;
diffuse radiation
ID PROBE WMAP OBSERVATIONS; POWER SPECTRUM ESTIMATION; POLARIZATION DATA;
SKY MAPS; FULL-SKY; MICROWAVE; PLANCK; PARAMETERS; VARIANCE; TEMPLATE
AB We present foreground-reduced cosmic microwave background (CMB) maps derived from the full Planck data set in both temperature and polarization. Compared to the corresponding Planck 2013 temperature sky maps, the total data volume is larger by a factor of 3.2 for frequencies between 30 and 70 GHz, and by 1.9 for frequencies between 100 and 857 GHz. In addition, systematic errors in the forms of temperature-topolarization leakage, analogue-to-digital conversion uncertainties, and very long time constant errors have been dramatically reduced, to the extent that the cosmological polarization signal may now be robustly recovered on angular scales l greater than or similar to 40. On the very largest scales, instrumental systematic residuals are still non-negligible compared to the expected cosmological signal, and modes with l < 20 are accordingly suppressed in the current polarization maps by high-pass filtering. As in 2013, four different CMB component separation algorithms are applied to these observations, providing a measure of stability with respect to algorithmic and modelling choices. The resulting polarization maps have rms instrumental noise ranging between 0.21 and 0.27 mu K averaged over 55' pixels, and between 4.5 and 6.1 mu K averaged over 3.'4 pixels. The cosmological parameters derived from the analysis of temperature power spectra are in agreement at the 1 sigma level with the Planck 2015 likelihood. Unresolved mismatches between the noise properties of the data and simulations prevent a satisfactory description of the higher-order statistical properties of the polarization maps. Thus, the primary applications of these polarization maps are those that do not require massive simulations for accurate estimation of uncertainties, for instance estimation of cross-spectra and cross-correlations, or stacking analyses. However, the amplitude of primordial non-Gaussianity is consistent with zero within 2 sigma for all local, equilateral, and orthogonal configurations of the bispectrum, including for polarization E-modes. Moreover, excellent agreement is found regarding the lensing B-mode power spectrum, both internally among the various component separation codes and with the best-fit Planck 2015 Lambda cold dark matter model.
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[Ade, P. A. R.; Munshi, D.; Spencer, L. D.; Sudiwala, R.] Cardiff Univ, Sch Phys & Astron, Queens Bldg, Cardiff CF24 3AA, S Glam, Wales.
[Moss, A.] Univ Nottingham, Sch Phys & Astron, Nottingham NG7 2RD, England.
[Bouchet, F. R.] Sorbonne Univ UPMC, Inst Astrophys Paris, UMR 7095, 98bis Blvd Arago, F-75014 Paris, France.
[Sunyaev, R.] Russian Acad Sci, Space Res Inst IKI, Profsoyuznaya Str 84-32, Moscow 117997, Russia.
[Borrill, J.] Univ Calif Berkeley, Space Sci Lab, Berkeley, CA 94720 USA.
[Stolyarov, V.] Russian Acad Sci, Special Astrophys Observ, Karachai Cherkessian Rep 369167, Zelenchukskiy R, Russia.
[Calabrese, E.] Univ Oxford, Subdept Astrophys, Keble Rd, Oxford OX1 3RH, England.
[Gudmundsson, J. E.] Stockholm Univ, Dept Phys, Oskar Klein Ctr Cosmoparticle Phys, AlbaNova, S-10691 Stockholm, Sweden.
[Lesgourgues, J.] CERN, PH TH, Div Theory, CH-1211 Geneva 23, Switzerland.
[Benabed, K.; Benoit-Levy, A.; Colombi, S.; Elsner, F.; Hivon, E.; Prunet, S.; Wandelt, B. D.] UPMC Univ Paris 06, UMR 7095, 98bis Blvd Arago, F-75014 Paris, France.
[Banday, A. J.; Bernard, J. -P.; Forni, O.; Giard, M.; Jaffe, T. R.; Montier, L.; Pointecouteau, E.; Ristorcelli, I.] Univ Toulouse, UPS OMP, IRAP, F-31028 Toulouse 4, France.
[Reach, W. T.] Univ Space Res Assoc, Stratospher Observ Infrared Astron, MS 232-11, Moffett Field, CA 94035 USA.
[Battaner, E.] Univ Granada, Dept Fis Teer & Cosmos, Fac Ciencias, E-18071 Granada, Spain.
[Battaner, E.] Univ Granada, Inst Carlos Fis Teor & Computac 1, Granada, Spain.
[Gorski, K. M.] Univ Warsaw Observ, Aleje Ujazdowskie 4, PL-00478 Warsaw, Poland.
RP Ashdown, M (reprint author), Univ Cambridge, Cavendish Lab, Astrophys Grp, JJ Thomson Ave, Cambridge CB3 0HE, England.; Ashdown, M (reprint author), Kavli Inst Cosmol Cambridge, Madingley Rd, Cambridge CB3 0HA, England.
EM maja1@mrao.cam.acuk
RI Barreiro, Rita Belen/N-5442-2014; bonavera, laura/E-9368-2017;
Gonzalez-Nuevo, Joaquin/I-3562-2014; Herranz, Diego/K-9143-2014;
Colombo, Loris/J-2415-2016;
OI Stolyarov, Vladislav/0000-0001-8151-828X; Barreiro, Rita
Belen/0000-0002-6139-4272; TERENZI, LUCA/0000-0001-9915-6379; bonavera,
laura/0000-0001-8039-3876; Reach, William/0000-0001-8362-4094;
Valiviita, Jussi/0000-0001-6225-3693; Hurier,
Guillaume/0000-0002-1215-0706; Gonzalez-Nuevo,
Joaquin/0000-0003-1354-6822; Herranz, Diego/0000-0003-4540-1417;
Colombo, Loris/0000-0003-4572-7732; Zacchei, Andrea/0000-0003-0396-1192;
Piacentini, Francesco/0000-0002-5444-9327; Molinari,
Diego/0000-0002-7799-3915; Toffolatti, Luigi/0000-0003-2645-7386; Lilje,
Per/0000-0003-4324-7794; Paoletti, Daniela/0000-0003-4761-6147; Nati,
Federico/0000-0002-8307-5088; Savini, Giorgio/0000-0003-4449-9416;
Pierpaoli, Elena/0000-0002-7957-8993
FU ESA; CNES (France); CNRS/INSU-IN2P3-INP (France); ASI (Italy); CNR
(Italy); INAF (Italy); NASA (USA); DoE (USA); STFC (UK); UKSA (UK); CSIC
(Spain); MINECO (Spain); JA (Spain); RES (Spain); Tekes (Finland); AoF
(Finland); CSC (Finland); DLR (Germany); MPG (Germany); CSA (Canada);
DTU Space (Denmark); SER/SSO (Switzerland); RCN (Norway); SFI (Ireland);
FCT/MCTES (Portugal); ERC (EU); PRACE (EU)
FX The Planck Collaboration acknowledges the support of: ESA; CNES, and
CNRS/INSU-IN2P3-INP (France); ASI, CNR, and INAF (Italy); NASA and DoE
(USA); STFC and UKSA (UK); CSIC, MINECO, JA and RES (Spain); Tekes, AoF,
and CSC (Finland); DLR and MPG (Germany); CSA (Canada); DTU Space
(Denmark); SER/SSO (Switzerland); RCN (Norway); SFI (Ireland); FCT/MCTES
(Portugal); ERC and PRACE (EU). A description of the Planck
Collaboration and a list of its members, indicating which technical or
scientific activities they have been involved in, can be found at
http://www.cosmos.esa.int/web/planck/planck-collaboration. Some of the
results in this paper have been derived using the HEALPix package.
NR 64
TC 5
Z9 5
U1 1
U2 1
PU EDP SCIENCES S A
PI LES ULIS CEDEX A
PA 17, AVE DU HOGGAR, PA COURTABOEUF, BP 112, F-91944 LES ULIS CEDEX A,
FRANCE
SN 1432-0746
J9 ASTRON ASTROPHYS
JI Astron. Astrophys.
PD OCT
PY 2016
VL 594
AR A9
DI 10.1051/0004-6361/201525936
PG 42
WC Astronomy & Astrophysics
SC Astronomy & Astrophysics
GA DZ4MG
UT WOS:000385832200019
ER
PT J
AU Adam, R
Ade, PAR
Aghanim, N
Akrami, Y
Alves, MIR
Argueso, F
Arnaud, M
Arroja, F
Ashdown, M
Aumont, J
Baccigalupi, C
Ballardini, M
Banday, AJ
Barreiro, RB
Bartlett, JG
Bartolo, N
Basak, S
Battaglia, P
Battaner, E
Battye, R
Benabed, K
Benoit, A
Benoit-Levy, A
Bernard, JP
Bersanelli, M
Bertincourt, B
Bielewicz, P
Bikmaev, I
Bock, JJ
Bohringer, H
Bonaldi, A
Bonavera, L
Bond, JR
Borrill, J
Bouchet, FR
Boulanger, F
Bucher, M
Burenin, R
Burigana, C
Butler, RC
Calabrese, E
Cardoso, JF
Carvalho, P
Casaponsa, B
Castex, G
Catalano, A
Challinor, A
Chamballu, A
Chary, RR
Chiang, HC
Chluba, J
Chon, G
Christensen, PR
Church, S
Clemens, M
Clements, DL
Colombi, S
Colombo, LPL
Combet, C
Comis, B
Contreras, D
Couchot, F
Coulais, A
Crill, BP
Cruz, M
Curto, A
Cuttaia, F
Danese, L
Davies, RD
Davis, RJ
de Bernardis, P
de Rosa, A
de Zotti, G
Delabrouille, J
Delouis, JM
Desert, FX
Di Valentino, E
Dickinson, C
Diego, JM
Dolag, K
Dole, H
Donzelli, S
Dore, O
Douspis, M
Ducout, A
Dunkley, J
Dupac, X
Efstathiou, G
Eisenhardt, PRM
Elsner, F
Ensslin, TA
Eriksen, HK
Falgarone, E
Fantaye, Y
Farhang, M
Feeney, S
Fergusson, J
Fernandez-Cobos, R
Feroz, F
Finelli, F
Florido, E
Forni, O
Frailis, M
Fraisse, AA
Franceschet, C
Franceschi, E
Frejsel, A
Frolov, A
Galeotta, S
Galli, S
Ganga, K
Gauthier, C
Genova-Santos, RT
Gerbino, M
Ghosh, T
Giard, M
Giraud-Heraud, Y
Giusarma, E
Gjerlow, E
Gonzalez-Nuevo, J
Gorski, KM
Grainge, KJB
Gratton, S
Gregorio, A
Gruppuso, A
Gudmundsson, JE
Hamann, J
Handley, W
Hansen, FK
Hanson, D
Harrison, DL
Heavens, A
Helou, G
Henrot-Versille, S
Hernandez-Monteagudo, C
Herranz, D
Hildebrandt, SR
Hivon, E
Hobson, M
Holmes, WA
Hornstrup, A
Hovest, W
Huang, Z
Huffenberger, KM
Hurier, G
Ilic, S
Jaffe, AH
Jaffe, TR
Jin, T
Jones, WC
Juvela, M
Karakci, A
Keihanen, E
Keskitalo, R
Khamitov, I
Kiiveri, K
Kim, J
Kisner, TS
Kneissl, R
Knoche, J
Knox, L
Krachmalnicoff, N
Kunz, M
Kurki-Suonio, H
Lacasa, F
Lagache, G
Lahteenmaki, A
Lamarre, JM
Langer, M
Lasenby, A
Lattanzi, M
Lawrence, CR
Jeune, M
Leahy, JP
Lellouch, E
Leonardi, R
Leon-Tavares, J
Lesgourgues, J
Levrier, F
Lewis, A
Liguori, M
Lilje, PB
Lilley, M
Linden-Vornle, M
Lindholm, V
Liu, H
Lopez-Caniego, M
Lubin, PM
Ma, YZ
Macias-Perez, JF
Maggio, G
Maino, D
Mak, DSY
Mandolesi, N
Mangilli, A
Marchini, A
Marcos-Caballero, A
Marinucci, D
Maris, M
Marshall, DJ
Martin, PG
Martinelli, M
Martinez-Gonzalez, E
Masi, S
Matarrese, S
Mazzotta, P
McEwen, JD
McGehee, P
Mei, S
Meinhold, PR
Melchiorri, A
Melin, JB
Mendes, L
Mennella, A
Migliaccio, M
Mikkelsen, K
Millea, M
Mitra, S
Miville-Deschenes, MA
Molinari, D
Moneti, A
Montier, L
Moreno, R
Morgante, G
Mortlock, D
Moss, A
Mottet, S
Munchmeyer, M
Munshi, D
Murphy, JA
Narimani, A
Naselsky, P
Nastasi, A
Nati, F
Natoli, P
Negrello, M
Netterfield, CB
Norgaard-Nielsen, HU
Noviello, F
Novikov, D
Novikov, I
Olamaie, M
Oppermann, N
Orlando, E
Oxborrow, CA
Paci, F
Pagano, L
Pajot, F
Paladini, R
Pandolfi, S
Paoletti, D
Partridge, B
Pasian, F
Patanchon, G
Pearson, TJ
Peel, M
Peiris, HV
Pelkonen, VM
Perdereau, O
Perotto, L
Perrott, YC
Perrotta, F
Pettorino, V
Piacentini, F
Piat, M
Pierpaoli, E
Pietrobon, D
Plaszczynski, S
Pogosyan, D
Pointecouteau, E
Polenta, G
Popa, L
Pratt, GW
Prezeau, G
Prunet, S
Puget, JL
Rachen, JP
Racine, B
Reach, WT
Rebolo, R
Reinecke, M
Remazeilles, M
Renault, C
Renzi, A
Ristorcelli, I
Rocha, G
Roman, M
Romelli, E
Rosset, C
Rossetti, M
Rotti, A
Roudier, G
d'Orfeuil, BR
Rowan-Robinson, M
Rubino-Martin, JA
Ruiz-Granados, B
Rumsey, C
Rusholme, B
Said, N
Salvatelli, V
Salvati, L
Sandri, M
Sanghera, HS
Santos, D
Saunders, RDE
Sauve, A
Savelainen, M
Savini, G
Schaefer, BM
Schammel, MP
Scott, D
Seiffert, MD
Serra, P
Shellard, EPS
Shimwell, TW
Shiraishi, M
Smith, K
Souradeep, T
Spencer, LD
Spinelli, M
Stanford, SA
Stern, D
Stolyarov, V
Stompor, R
Strong, AW
Sudiwala, R
Sunyaev, R
Sutter, P
Sutton, D
Suur-Uski, AS
Sygnet, JF
Tauber, JA
Tavagnacco, D
Terenzi, L
Texier, D
Toffolatti, L
Tomasi, M
Tornikoski, M
Tramonte, D
Tristram, M
Troja, A
Trombetti, T
Tucci, M
Tuovinen, J
Turler, M
Umana, G
Valenziano, L
Valiviita, J
Van Tent, F
Vassallo, T
Vibert, L
Vidal, M
Viel, M
Vielva, P
Villa, F
Wade, LA
Walter, B
Wandelt, BD
Watson, R
Wehus, IK
Welikala, N
Weller, J
White, M
White, SDM
Wilkinson, A
Yvon, D
Zacchei, A
Zibin, JP
Zonca, A
AF Adam, R.
Ade, P. A. R.
Aghanim, N.
Akrami, Y.
Alves, M. I. R.
Argueeso, F.
Arnaud, M.
Arroja, F.
Ashdown, M.
Aumont, J.
Baccigalupi, C.
Ballardini, M.
Banday, A. J.
Barreiro, R. B.
Bartlett, J. G.
Bartolo, N.
Basak, S.
Battaglia, P.
Battaner, E.
Battye, R.
Benabed, K.
Benoit, A.
Benoit-Levy, A.
Bernard, J. -P.
Bersanelli, M.
Bertincourt, B.
Bielewicz, P.
Bikmaev, I.
Bock, J. J.
Boehringer, H.
Bonaldi, A.
Bonavera, L.
Bond, J. R.
Borrill, J.
Bouchet, F. R.
Boulanger, F.
Bucher, M.
Burenin, R.
Burigana, C.
Butler, R. C.
Calabrese, E.
Cardoso, J. -F.
Carvalho, P.
Casaponsa, B.
Castex, G.
Catalano, A.
Challinor, A.
Chamballu, A.
Chary, R. -R.
Chiang, H. C.
Chluba, J.
Chon, G.
Christensen, P. R.
Church, S.
Clemens, M.
Clements, D. L.
Colombi, S.
Colombo, L. P. L.
Combet, C.
Comis, B.
Contreras, D.
Couchot, F.
Coulais, A.
Crill, B. P.
Cruz, M.
Curto, A.
Cuttaia, F.
Danese, L.
Davies, R. D.
Davis, R. J.
de Bernardis, P.
de Rosa, A.
de Zotti, G.
Delabrouille, J.
Delouis, J. -M.
Desert, F. -X.
Di Valentino, E.
Dickinson, C.
Diego, J. M.
Dolag, K.
Dole, H.
Donzelli, S.
Dore, O.
Douspis, M.
Ducout, A.
Dunkley, J.
Dupac, X.
Efstathiou, G.
Eisenhardt, P. R. M.
Elsner, F.
Ensslin, T. A.
Eriksen, H. K.
Falgarone, E.
Fantaye, Y.
Farhang, M.
Feeney, S.
Fergusson, J.
Fernandez-Cobos, R.
Feroz, F.
Finelli, F.
Florido, E.
Forni, O.
Frailis, M.
Fraisse, A. A.
Franceschet, C.
Franceschi, E.
Frejsel, A.
Frolov, A.
Galeotta, S.
Galli, S.
Ganga, K.
Gauthier, C.
Genova-Santos, R. T.
Gerbino, M.
Ghosh, T.
Giard, M.
Giraud-Heraud, Y.
Giusarma, E.
Gjerlow, E.
Gonzalez-Nuevo, J.
Gorski, K. M.
Grainge, K. J. B.
Gratton, S.
Gregorio, A.
Gruppuso, A.
Gudmundsson, J. E.
Hamann, J.
Handley, W.
Hansen, F. K.
Hanson, D.
Harrison, D. L.
Heavens, A.
Helou, G.
Henrot-Versille, S.
Hernandez-Monteagudo, C.
Herranz, D.
Hildebrandt, S. R.
Hivon, E.
Hobson, M.
Holmes, W. A.
Hornstrup, A.
Hovest, W.
Huang, Z.
Huffenberger, K. M.
Hurier, G.
Ilic, S.
Jaffe, A. H.
Jaffe, T. R.
Jin, T.
Jones, W. C.
Juvela, M.
Karakci, A.
Keihanen, E.
Keskitalo, R.
Khamitov, I.
Kiiveri, K.
Kim, J.
Kisner, T. S.
Kneissl, R.
Knoche, J.
Knox, L.
Krachmalnicoff, N.
Kunz, M.
Kurki-Suonio, H.
Lacasa, F.
Lagache, G.
Lahteenmaki, A.
Lamarre, J. -M.
Langer, M.
Lasenby, A.
Lattanzi, M.
Lawrence, C. R.
Le Jeune, M.
Leahy, J. P.
Lellouch, E.
Leonardi, R.
Leon-Tavares, J.
Lesgourgues, J.
Levrier, F.
Lewis, A.
Liguori, M.
Lilje, P. B.
Lilley, M.
Linden-Vornle, M.
Lindholm, V.
Liu, H.
Lopez-Caniego, M.
Lubin, P. M.
Ma, Y. -Z.
Macias-Perez, J. F.
Maggio, G.
Maino, D.
Mak, D. S. Y.
Mandolesi, N.
Mangilli, A.
Marchini, A.
Marcos-Caballero, A.
Marinucci, D.
Maris, M.
Marshall, D. J.
Martin, P. G.
Martinelli, M.
Martinez-Gonzalez, E.
Masi, S.
Matarrese, S.
Mazzotta, P.
McEwen, J. D.
McGehee, P.
Mei, S.
Meinhold, P. R.
Melchiorri, A.
Melin, J. -B.
Mendes, L.
Mennella, A.
Migliaccio, M.
Mikkelsen, K.
Millea, M.
Mitra, S.
Miville-Deschenes, M. -A.
Molinari, D.
Moneti, A.
Montier, L.
Moreno, R.
Morgante, G.
Mortlock, D.
Moss, A.
Mottet, S.
Muenchmeyer, M.
Munshi, D.
Murphy, J. A.
Narimani, A.
Naselsky, P.
Nastasi, A.
Nati, F.
Natoli, P.
Negrello, M.
Netterfield, C. B.
Norgaard-Nielsen, H. U.
Noviello, F.
Novikov, D.
Novikov, I.
Olamaie, M.
Oppermann, N.
Orlando, E.
Oxborrow, C. A.
Paci, F.
Pagano, L.
Pajot, F.
Paladini, R.
Pandolfi, S.
Paoletti, D.
Partridge, B.
Pasian, F.
Patanchon, G.
Pearson, T. J.
Peel, M.
Peiris, H. V.
Pelkonen, V. -M.
Perdereau, O.
Perotto, L.
Perrott, Y. C.
Perrotta, F.
Pettorino, V.
Piacentini, F.
Piat, M.
Pierpaoli, E.
Pietrobon, D.
Plaszczynski, S.
Pogosyan, D.
Pointecouteau, E.
Polenta, G.
Popa, L.
Pratt, G. W.
Prezeau, G.
Prunet, S.
Puget, J. -L.
Rachen, J. P.
Racine, B.
Reach, W. T.
Rebolo, R.
Reinecke, M.
Remazeilles, M.
Renault, C.
Renzi, A.
Ristorcelli, I.
Rocha, G.
Roman, M.
Romelli, E.
Rosset, C.
Rossetti, M.
Rotti, A.
Roudier, G.
d'Orfeuil, B. Rouille
Rowan-Robinson, M.
Rubino-Martin, J. A.
Ruiz-Granados, B.
Rumsey, C.
Rusholme, B.
Said, N.
Salvatelli, V.
Salvati, L.
Sandri, M.
Sanghera, H. S.
Santos, D.
Saunders, R. D. E.
Sauve, A.
Savelainen, M.
Savini, G.
Schaefer, B. M.
Schammel, M. P.
Scott, D.
Seiffert, M. D.
Serra, P.
Shellard, E. P. S.
Shimwell, T. W.
Shiraishi, M.
Smith, K.
Souradeep, T.
Spencer, L. D.
Spinelli, M.
Stanford, S. A.
Stern, D.
Stolyarov, V.
Stompor, R.
Strong, A. W.
Sudiwala, R.
Sunyaev, R.
Sutter, P.
Sutton, D.
Suur-Uski, A. -S.
Sygnet, J. -F.
Tauber, J. A.
Tavagnacco, D.
Terenzi, L.
Texier, D.
Toffolatti, L.
Tomasi, M.
Tornikoski, M.
Tramonte, D.
Tristram, M.
Troja, A.
Trombetti, T.
Tucci, M.
Tuovinen, J.
Turler, M.
Umana, G.
Valenziano, L.
Valiviita, J.
Van Tent, F.
Vassallo, T.
Vibert, L.
Vidal, M.
Viel, M.
Vielva, P.
Villa, F.
Wade, L. A.
Walter, B.
Wandelt, B. D.
Watson, R.
Wehus, I. K.
Welikala, N.
Weller, J.
White, M.
White, S. D. M.
Wilkinson, A.
Yvon, D.
Zacchei, A.
Zibin, J. P.
Zonca, A.
CA Planck Collaboration
TI Planck 2015 results I. Overview of products and scientific results
SO ASTRONOMY & ASTROPHYSICS
LA English
DT Article
DE cosmology: observations; cosmic background radiation; surveys; space
vehicles: instruments; instrumentation: detectors
ID ANGULAR POWER SPECTRUM; PROBE WMAP OBSERVATIONS; MICROWAVE BACKGROUND
TEMPERATURE; PRE-LAUNCH STATUS; COMPONENT SEPARATION; SKY MAPS;
INTERSTELLAR DUST; POLARIZATION DATA; MAGNETIC-FIELD; ANISOTROPY
AB The European Space Agency's Planck satellite, which is dedicated to studying the early Universe and its subsequent evolution, was launched on 14 May 2009. It scanned the microwave and submillimetre sky continuously between 12 August 2009 and 23 October 2013. In February 2015, ESA and the Planck Collaboration released the second set of cosmology products based on data from the entire Planck mission, including both temperature and polarization, along with a set of scientific and technical papers and a web-based explanatory supplement. This paper gives an overview of the main characteristics of the data and the data products in the release, as well as the associated cosmological and astrophysical science results and papers. The data products include maps of the cosmic microwave background (CMB), the thermal Sunyaev-Zeldovich effect, diffuse foregrounds in temperature and polarization, catalogues of compact Galactic and extragalactic sources (including separate catalogues of Sunyaev-Zeldovich clusters and Galactic cold clumps), and extensive simulations of signals and noise used in assessing uncertainties and the performance of the analysis methods. The likelihood code used to assess cosmological models against the Planck data is described, along with a CMB lensing likelihood. Scientific results include cosmological parameters derived from CMB power spectra, gravitational lensing, and cluster counts, as well as constraints on inflation, non-Gaussianity, primordial magnetic fields, dark energy, and modified gravity, and new results on low-frequency Galactic foregrounds.
C1 [Bartlett, J. G.; Bucher, M.; Cardoso, J. -F.; Castex, G.; Delabrouille, J.; Ganga, K.; Gauthier, C.; Giraud-Heraud, Y.; Karakci, A.; Le Jeune, M.; Patanchon, G.; Piat, M.; Remazeilles, M.; Roman, M.; Rosset, C.; Roudier, G.; Stompor, R.] Univ Paris Diderot, APC AstroParticule & Cosmol, CNRS IN2P3, CEA Irfu,Observ Paris,Sorbonne Paris Cite, 10 Rue Alice Domon & Leonie Duquet, F-75205 Paris 13, France.
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RP Lawrence, CR (reprint author), CALTECH, Jet Prop Lab, 4800 Oak Grove Dr, Pasadena, CA 91109 USA.
EM charles.lawrence@jpl.nasa.gov
RI Lahteenmaki, Anne/L-5987-2013; Gerbino, Martina/E-4029-2017; Barreiro,
Rita Belen/N-5442-2014; Mazzotta, Pasquale/B-1225-2016; bonavera,
laura/E-9368-2017; Gonzalez-Nuevo, Joaquin/I-3562-2014; Herranz,
Diego/K-9143-2014; Colombo, Loris/J-2415-2016;
OI Savini, Giorgio/0000-0003-4449-9416; Martinelli,
Matteo/0000-0002-6943-7732; Pierpaoli, Elena/0000-0002-7957-8993;
Juvela, Mika/0000-0002-5809-4834; Paoletti, Daniela/0000-0003-4761-6147;
Huang, Zhiqi/0000-0002-1506-1063; TERENZI, LUCA/0000-0001-9915-6379;
Reach, William/0000-0001-8362-4094; Valiviita,
Jussi/0000-0001-6225-3693; Kurki-Suonio, Hannu/0000-0002-4618-3063;
Molinari, Diego/0000-0002-7799-3915; Toffolatti,
Luigi/0000-0003-2645-7386; Nati, Federico/0000-0002-8307-5088;
Stolyarov, Vladislav/0000-0001-8151-828X; Gerbino,
Martina/0000-0002-3538-1283; Barreiro, Rita Belen/0000-0002-6139-4272;
Mazzotta, Pasquale/0000-0002-5411-1748; bonavera,
laura/0000-0001-8039-3876; Gonzalez-Nuevo, Joaquin/0000-0003-1354-6822;
Herranz, Diego/0000-0003-4540-1417; Colombo, Loris/0000-0003-4572-7732;
Liu, Hao/0000-0003-4410-5827; Hivon, Eric/0000-0003-1880-2733; Zacchei,
Andrea/0000-0003-0396-1192
FU CNES; CNRS/INSU-IN2P3; ASI; Danish Natural Research Council; ESA; CNES
(France); CNRS/INSU-IN2P3INP (France); ASI (Italy); CNR (Italy); INAF
(Italy); NASA (USA); DoE (USA); STFC (UK); UKSA (UK); CSIC (Spain);
MINECO (Spain); JA (Spain); RES (Spain); Tekes (Finland); AoF (Finland);
CSC (Finland); DLR (Germany); MPG (Germany); CSA (Canada); DTU Space
(Denmark); SER/SSO (Switzerland); RCN (Norway); SFI (Ireland); FCT/MCTES
(Portugal); ERC (EU); PRACE (EU); LFI; HFI
FX Planck is a project of the European Space Agency in cooperation with the
scientific community, which started in 1993. ESA led the project,
developed the satellite, integrated the payload into it, and launched
and operated the satellite. Two Consortia, comprising around 100
scientific institutes within Europe, the USA, and Canada, and funded by
agencies from the participating countries, developed and operated the
scientific instruments LFI and HFI. The Consortia are also responsible
for scientific processing of the acquired data. The Consortia are led by
the Principal Investigators: J.-L. Puget in France for HFI (funded
principally by CNES and CNRS/INSU-IN2P3) and N. Mandolesi in Italy for
LFI (funded principally via ASI). NASA's US Planck Project, based at JPL
and involving scientists at many US institutions, contributes
significantly to the efforts of these two Consortia. A third Consortium,
led by H.U. Norgaard-Nielsen and supported by the Danish Natural
Research Council, contributed to the reflector programme. These three
Consortia, together with ESA's Planck Science Office, form the Planck
Collaboration. A description of the Planck Collaboration and a list of
its members, indicating which technical or scientific activities they
have been involved in, can be found at
http://www.cosmos.esa.int/web/planck/planck-collaboration. The Planck
Collaboration acknowledges the support of: ESA; CNES and
CNRS/INSU-IN2P3INP (France); ASI, CNR, and INAF (Italy); NASA and DoE
(USA); STFC and UKSA (UK); CSIC, MINECO, JA, and RES (Spain); Tekes,
AoF, and CSC (Finland); DLR and MPG (Germany); CSA (Canada); DTU Space
(Denmark); SER/SSO (Switzerland); RCN (Norway); SFI (Ireland); FCT/MCTES
(Portugal); ERC and PRACE (EU). We thank Diego Falceta-Goncalves for
providing the technique for making the line-integral-convolution maps
presented in Figs. 23 and 25.
NR 127
TC 16
Z9 16
U1 1
U2 1
PU EDP SCIENCES S A
PI LES ULIS CEDEX A
PA 17, AVE DU HOGGAR, PA COURTABOEUF, BP 112, F-91944 LES ULIS CEDEX A,
FRANCE
SN 1432-0746
J9 ASTRON ASTROPHYS
JI Astron. Astrophys.
PD OCT
PY 2016
VL 594
AR A1
DI 10.1051/0004-6361/201527101
PG 38
WC Astronomy & Astrophysics
SC Astronomy & Astrophysics
GA DZ4MG
UT WOS:000385832200030
ER
PT J
AU Ade, PAR
Aghanim, N
Arnaud, M
Ashdown, M
Aumont, J
Baccigalupi, C
Banday, AJ
Barreiro, RB
Bartlett, JG
Bartolo, N
Battaner, E
Benabed, K
Benoit, A
Benoit-Levy, A
Bernard, JP
Bersanelli, M
Bielewicz, P
Bock, JJ
Bonaldi, A
Bonavera, L
Bond, JR
Borrill, J
Bouchet, FR
Boulanger, F
Bucher, M
Burigana, C
Butler, RC
Calabrese, E
Cardoso, JF
Castex, G
Catalano, A
Challinor, A
Chamballu, A
Chiang, HC
Christensen, PR
Clements, DL
Colombi, S
Colombo, LPL
Combet, C
Couchot, F
Coulais, A
Crill, BP
Curto, A
Cuttaia, F
Danese, L
Davies, RD
Davis, RJ
de Bernardis, P
de Rosa, A
de Zotti, G
Delabrouille, J
Delouis, JM
Desert, FX
Dickinson, C
Diego, JM
Dolag, K
Dole, H
Donzelli, S
Dore, O
Douspis, M
Ducout, A
Dupac, X
Efstathiou, G
Elsner, F
Ensslin, TA
Eriksen, HK
Fergusson, J
Finelli, F
Forni, O
Frailis, M
Fraisse, AA
Franceschi, E
Frejsel, A
Galeotta, S
Galli, S
Ganga, K
Ghosh, T
Giard, M
Giraud-Heraud, Y
Gjerlow, E
Gonzalez-Nuevo, J
Gorski, KM
Gratton, S
Gregorio, A
Gruppuso, A
Gudmundsson, JE
Hansen, FK
Hanson, D
Harrison, DL
Henrot-Versille, S
Hernandez-Monteagudo, C
Herranz, D
Hildebrandt, SR
Hivon, E
Hobson, M
Holmes, WA
Hornstrup, A
Hovest, W
Huffenberger, KM
Hurier, G
Jaffe, AH
Jaffe, TR
Jones, WC
Juvela, M
Karakei, A
Keihanen, E
Keskitalo, R
Kiiveri, K
Kisner, TS
Kneissl, R
Knoche, J
Kunz, M
Kurki-Suonio, H
Lagache, G
Lamarre, JM
Lasenby, A
Lattanzi, M
Lawrence, CR
Leonardi, R
Lesgourgues, J
Levrier, F
Liguori, M
Lilje, PB
Linden-Vornle, M
Lindholm, V
Lopez-Caniego, M
Lubin, PM
Macias-Perez, JF
Maggio, G
Maino, D
Mandolesi, N
Mangilli, A
Maris, M
Martin, PG
Martinez-Gonzalez, E
Masi, S
Matarrese, S
McGehee, P
Meinhold, PR
Melchiorri, A
Melin, JB
Mendes, L
Mennella, A
Migliaccio, M
Mitra, S
Miville-Deschenes, MA
Moneti, A
Montier, L
Morgante, G
Mortlock, D
Moss, A
Munshi, D
Murphy, JA
Naselsky, P
Nati, F
Natoli, P
Netterfield, CB
Norgaard-Nielsen, HU
Noviello, F
Novikov, D
Novikov, I
Oxborrow, CA
Paci, F
Pagano, L
Pajot, F
Paoletti, D
Pasian, F
Patanchon, G
Pearson, TJ
Perdereau, O
Perotto, L
Perrotta, F
Pettorino, V
Piacentini, F
Piat, M
Pierpaoli, E
Pietrobon, D
Plaszczynski, S
Pointecouteau, E
Polenta, G
Pratt, GW
Prezeau, G
Prunet, S
Puget, JL
Rachen, JP
Rebolo, R
Reinecke, M
Remazeilles, M
Renault, C
Renzi, A
Ristorcelli, I
Rocha, G
Roman, M
Rosset, C
Rossetti, M
Roudier, G
Rubino-Martin, JA
Rusholme, B
Sandri, M
Santos, D
Savelainen, M
Scott, D
Seiffert, MD
Shellard, EPS
Spencer, LD
Stolyarov, V
Stompor, R
Sudiwala, R
Sutton, D
Suur-Uski, AS
Sygnet, JF
Tauber, JA
Terenzi, L
Toffolatti, L
Tomasi, M
Tristram, M
Tucci, M
Tuovinen, J
Valenziano, L
Valiviita, J
Van Tent, B
Vielva, P
Villa, F
Wade, LA
Wandelt, BD
Wehus, IK
Welikala, N
Yvon, D
Zacchei, A
Zonca, A
AF Ade, P. A. R.
Aghanim, N.
Arnaud, M.
Ashdown, M.
Aumont, J.
Baccigalupi, C.
Banday, A. J.
Barreiro, R. B.
Bartlett, J. G.
Bartolo, N.
Battaner, E.
Benabed, K.
Benoit, A.
Benoit-Levy, A.
Bernard, J. -P.
Bersanelli, M.
Bielewicz, P.
Bock, J. J.
Bonaldi, A.
Bonavera, L.
Bond, J. R.
Borrill, J.
Bouchet, F. R.
Boulanger, F.
Bucher, M.
Burigana, C.
Butler, R. C.
Calabrese, E.
Cardoso, J. -F.
Castex, G.
Catalano, A.
Challinor, A.
Chamballu, A.
Chiang, H. C.
Christensen, P. R.
Clements, D. L.
Colombi, S.
Colombo, L. P. L.
Combet, C.
Couchot, F.
Coulais, A.
Crill, B. P.
Curto, A.
Cuttaia, F.
Danese, L.
Davies, R. D.
Davis, R. J.
de Bernardis, P.
de Rosa, A.
de Zotti, G.
Delabrouille, J.
Delouis, J. -M.
Desert, F. -X.
Dickinson, C.
Diego, J. M.
Dolag, K.
Dole, H.
Donzelli, S.
Dore, O.
Douspis, M.
Ducout, A.
Dupac, X.
Efstathiou, G.
Elsner, F.
Ensslin, T. A.
Eriksen, H. K.
Fergusson, J.
Finelli, F.
Forni, O.
Frailis, M.
Fraisse, A. A.
Franceschi, E.
Frejsel, A.
Galeotta, S.
Galli, S.
Ganga, K.
Ghosh, T.
Giard, M.
Giraud-Heraud, Y.
Gjerlow, E.
Gonzalez-Nuevo, J.
Gorski, K. M.
Gratton, S.
Gregorio, A.
Gruppuso, A.
Gudmundsson, J. E.
Hansen, F. K.
Hanson, D.
Harrison, D. L.
Henrot-Versille, S.
Hernandez-Monteagudo, C.
Herranz, D.
Hildebrandt, S. R.
Hivon, E.
Hobson, M.
Holmes, W. A.
Hornstrup, A.
Hovest, W.
Huffenberger, K. M.
Hurier, G.
Jaffe, A. H.
Jaffe, T. R.
Jones, W. C.
Juvela, M.
Karakei, A.
Keihanen, E.
Keskitalo, R.
Kiiveri, K.
Kisner, T. S.
Kneissl, R.
Knoche, J.
Kunz, M.
Kurki-Suonio, H.
Lagache, G.
Lamarre, J. -M.
Lasenby, A.
Lattanzi, M.
Lawrence, C. R.
Leonardi, R.
Lesgourgues, J.
Levrier, F.
Liguori, M.
Lilje, P. B.
Linden-Vornle, M.
Lindholm, V.
Lopez-Caniego, M.
Lubin, P. M.
Macias-Perez, J. F.
Maggio, G.
Maino, D.
Mandolesi, N.
Mangilli, A.
Maris, M.
Martin, P. G.
Martinez-Gonzalez, E.
Masi, S.
Matarrese, S.
McGehee, P.
Meinhold, P. R.
Melchiorri, A.
Melin, J. -B.
Mendes, L.
Mennella, A.
Migliaccio, M.
Mitra, S.
Miville-Deschenes, M. -A.
Moneti, A.
Montier, L.
Morgante, G.
Mortlock, D.
Moss, A.
Munshi, D.
Murphy, J. A.
Naselsky, P.
Nati, F.
Natoli, P.
Netterfield, C. B.
Norgaard-Nielsen, H. U.
Noviello, F.
Novikov, D.
Novikov, I.
Oxborrow, C. A.
Paci, F.
Pagano, L.
Pajot, F.
Paoletti, D.
Pasian, F.
Patanchon, G.
Pearson, T. J.
Perdereau, O.
Perotto, L.
Perrotta, F.
Pettorino, V.
Piacentini, F.
Piat, M.
Pierpaoli, E.
Pietrobon, D.
Plaszczynski, S.
Pointecouteau, E.
Polenta, G.
Pratt, G. W.
Prezeau, G.
Prunet, S.
Puget, J. -L.
Rachen, J. P.
Rebolo, R.
Reinecke, M.
Remazeilles, M.
Renault, C.
Renzi, A.
Ristorcelli, I.
Rocha, G.
Roman, M.
Rosset, C.
Rossetti, M.
Roudier, G.
Rubino-Martin, J. A.
Rusholme, B.
Sandri, M.
Santos, D.
Savelainen, M.
Scott, D.
Seiffert, M. D.
Shellard, E. P. S.
Spencer, L. D.
Stolyarov, V.
Stompor, R.
Sudiwala, R.
Sutton, D.
Suur-Uski, A. -S.
Sygnet, J. -F.
Tauber, J. A.
Terenzi, L.
Toffolatti, L.
Tomasi, M.
Tristram, M.
Tucci, M.
Tuovinen, J.
Valenziano, L.
Valiviita, J.
Van Tent, B.
Vielva, P.
Villa, F.
Wade, L. A.
Wandelt, B. D.
Wehus, I. K.
Welikala, N.
Yvon, D.
Zacchei, A.
Zonca, A.
CA Planck Collaboration
TI Planck 2015 results XII. Full focal plane simulations
SO ASTRONOMY & ASTROPHYSICS
LA English
DT Article
DE methods: data analysis; methods: numerical; cosmic background radiation
ID MICROWAVE-ANISOTROPY-PROBE; STATISTICAL PROPERTIES; GALAXY CLUSTERS;
BACKGROUND MAPS; SPINNING DUST; SKY MAPS; EMISSION; CATALOG; SEPARATION;
MODEL
AB We present the 8th full focal plane simulation set (FFP8), deployed in support of the Planck 2015 results. FFP8 consists of 10 fiducial mission realizations reduced to 18 144 maps, together with the most massive suite of Monte Carlo realizations of instrument noise and CMB ever generated, comprising 104 mission realizations reduced to about 106 maps. The resulting maps incorporate the dominant instrumental, scanning, and data analysis effects, and the remaining subdominant effects will be included in future updates. Generated at a cost of some 25 million CPU-hours spread across multiple high-performance-computing (HPC) platforms, FFP8 is used to validate and verify analysis algorithms and their implementations, and to remove biases from and quantify uncertainties in the results of analyses of the real data.
C1 [Bartlett, J. G.; Bucher, M.; Cardoso, J. -F.; Castex, G.; Delabrouille, J.; Ganga, K.; Giraud-Heraud, Y.; Karakei, A.; Patanchon, G.; Piat, M.; Remazeilles, M.; Roman, M.; Rosset, C.; Roudier, G.; Stompor, R.] Univ Paris Diderot, APC AstroParticule & Cosmol, CNRS IN2P3, CEA Irfu,Observ Paris,Sorbonne Paris Cite, 10 Rue Alice Domon & Leonie Duquet, F-75205 Paris 13, France.
[Kunz, M.] African Inst Math Sci, 6-8 Melrose Rd, ZA-7945 Cape Town, South Africa.
[Natoli, P.; Polenta, G.] Agenzia Spaziale Italiana Sci Data Ctr, Via Politecn Snc, I-00133 Rome, Italy.
[Lagache, G.] Aix Marseille Univ, CNRS, LAM Lab Astrophys Marseille, UMR 7326, F-13388 Marseille, France.
[Ashdown, M.; Curto, A.; Hobson, M.; Lasenby, A.; Stolyarov, V.] Univ Cambridge, Cavendish Lab, Astrophys Grp, JJ Thomson Ave, Cambridge CB3 0HE, England.
[Chiang, H. C.] Univ KwaZulu Natal, Sch Math Stat & Comp Sci, Astrophys & Cosmol Res Unit, Westville Campus,Private Bag X54001, ZA-4000 Durban, South Africa.
[Kneissl, R.] ALMA Santiago Cent Off, Atacama Large Millimeter Submillimeter Array, Alonso de Cordova 3107,Vitacura,Casilla 763 0355, Santiago, Chile.
[Bond, J. R.; Hanson, D.; Martin, P. G.; Miville-Deschenes, M. -A.] Univ Toronto, CITA, 60 St George St, Toronto, ON M5S 3H8, Canada.
[Banday, A. J.; Bernard, J. -P.; Bielewicz, P.; Forni, O.; Giard, M.; Jaffe, T. R.; Montier, L.; Pointecouteau, E.; Ristorcelli, I.] CNRS, IRAP, 9 Av Colonel Roche,BP 44346, F-31028 Toulouse 4, France.
[Tuovinen, J.] Trinity Coll Dublin, CRANN, 91125 Dublin, Ireland.
[Bock, J. J.; Crill, B. P.; Dore, O.; Hildebrandt, S. R.; Pearson, T. J.; Prezeau, G.; Rocha, G.; Seiffert, M. D.] CALTECH, Pasadena, CA 91125 USA.
[Challinor, A.; Fergusson, J.; Shellard, E. P. S.] Univ Cambridge, Ctr Theoret Cosmol, DAMTP, Wilberforce Rd, Cambridge CB3 0WA, England.
[Hernandez-Monteagudo, C.] CEFCA, Plaza San Juan 1,Planta 2, Teruel 44001, Spain.
[Borrill, J.; Keskitalo, R.] Lawrence Berkeley Natl Lab, Computat Cosmol Ctr, Berkeley, CA 92093 USA.
[Rebolo, R.] CSIC, Madrid 0424, Spain.
[Chamballu, A.; Melin, J. -B.; Yvon, D.] CEA Saclay, DSM Irfu SPP, F-91191 Gif Sur Yvette, France.
[Hornstrup, A.; Linden-Vornle, M.] Tech Univ Denmark, Natl Space Inst, DTU Space, Elektrovej 327, DK-2800 Lyngby, Denmark.
[Kunz, M.; Tucci, M.] Univ Geneva, Dept Phys Theor, 24 Quai E Ansermet, CH-1211 Geneva 4, Switzerland.
[Rebolo, R.; Rubino-Martin, J. A.] Univ La Laguna ULL, Dept Astrofis, San Cristobal la Laguna 38206, Tenerife, Spain.
[Gonzalez-Nuevo, J.; Toffolatti, L.] Univ Oviedo, Dept Fis, Avda Calvo Sotelo S-N, E-33007 Oviedo, Spain.
[Netterfield, C. B.] Univ Toronto, Dept Astron & Astrophys, 50 St George St, Toronto, ON M5S 3H4, Canada.
[Rachen, J. P.] Radboud Univ Nijmegen, IMAPP, Dept Astrophys, POB 9010, NL-6500 GL Nijmegen, Netherlands.
[Scott, D.] Univ British Columbia, Dept Phys & Astron, 6224 Agr Rd, Vancouver, BC, Canada.
[Colombo, L. P. L.; Pierpaoli, E.] Univ Southern Calif, Dept Phys & Astron, Dana & David Dornsife Coll Letter Arts & Sci, Los Angeles, CA 90089 USA.
[Benoit-Levy, A.; Elsner, F.] UCL, Dept Phys & Astron, London WC1E 6BT, England.
[Huffenberger, K. M.] Florida State Univ, Dept Phys, Keen Phys Bldg,77 Chieftan Way, Tallahassee, FL 32306 USA.
[Juvela, M.; Keihanen, E.; Kiiveri, K.; Kurki-Suonio, H.; Lindholm, V.; Savelainen, M.; Suur-Uski, A. -S.; Valiviita, J.] Univ Helsinki, Dept Phys, Gustaf Hallstromin Katu 2a, Helsinki 00560, Finland.
[Chiang, H. C.; Fraisse, A. A.; Gudmundsson, J. E.; Jones, W. C.; Nati, F.] Princeton Univ, Dept Phys, Princeton, CA 93106 USA.
[Lubin, P. M.; Meinhold, P. R.; Zonca, A.] Univ Calif Santa Barbara, Dept Phys, Santa Barbara, CA 93106 USA.
[Wandelt, B. D.] Univ Illinois, Dept Phys, 1110 West Green St, Urbana, IL USA.
[Bartolo, N.; Liguori, M.; Matarrese, S.] Univ Padua, Dipartimento Fis & Astron G Galilei, Via Marzolo 8, I-35131 Padua, Italy.
[Burigana, C.; Lattanzi, M.; Mandolesi, N.; Natoli, P.] Univ Ferrara, Dipartimento Fis & Sci Terra, Via Saragat 1, I-44122 Ferrara, Italy.
[de Bernardis, P.; Masi, S.; Melchiorri, A.; Pagano, L.; Piacentini, F.] Univ Roma La Sapienza, Dipartimento Fis, Ple A Moro 2, I-00133 Rome, Italy.
[Bersanelli, M.; Maino, D.; Mennella, A.; Rossetti, M.; Tomasi, M.] Univ Milan, Dipartimento Fis, Via Celoria 16, I-00133 Milan, Italy.
[Gregorio, A.] Univ Trieste, Dipartimento Fis, Via A Valerio 2, I-34127 Trieste, Italy.
[Renzi, A.] Univ Roma Tor Vergata, Dipartimento Matemat, Via Ric Sci 1, I-000138 Rome, Italy.
[Christensen, P. R.; Naselsky, P.] Niels Bohr Inst, Discovery Ctr, Blegdamsvej 17, DK-1165 Copenhagen, Denmark.
[Kneissl, R.] European Southern Observ ESO Vitacura, Alonso de Cordova 3107,Casilla 19001, Santiago, Chile.
[Dupac, X.; Leonardi, R.; Lopez-Caniego, M.; Mendes, L.] European Space Agcy ESAC, Planck Sci Off, Camino Bajo del Castillo S-N, Madrid 28692, Spain.
[Tauber, J. A.] ESTEC, European Space Agcy, Keplerlaan 1, NL-2201 AZ Noordwijk, Netherlands.
[Terenzi, L.] Univ E Campus, Fac Ingn, Via Isimbardi 10, I-22060 Novedrate, CO, Italy.
[Matarrese, S.] INFN, Gran Sasso Sci Inst, Viale F Crispi 7, I-67100 Laquila, Italy.
[Pettorino, V.] HGSFP, Philosophenweg 16, D-69120 Heidelberg, Germany.
[Pettorino, V.] Heidelberg Univ, Dept Theoret Phys, Philosophenweg 16, D-69120 Heidelberg, Germany.
[Kiiveri, K.; Kurki-Suonio, H.; Lindholm, V.; Savelainen, M.; Suur-Uski, A. -S.; Valiviita, J.] Univ Helsinki, Helsinki Inst Phys, Gustaf Hallstromin Katu 2, Helsinki 00560, Finland.
[de Zotti, G.] Osserv Astron Padova, INAF, Vicolo Osservatorio 5, I-35131 Padua, Italy.
[Polenta, G.] Osservatorio Astronom Roma, INAF, Via Frascati 33, Monte Porzio Catone, Italy.
[Frailis, M.; Galeotta, S.; Gregorio, A.; Maggio, G.; Maris, M.; Pasian, F.; Zacchei, A.] Osservatorio Astronom Trieste, INAF, Via GB Tiepolo 11, I-34127 Trieste, Italy.
[Burigana, C.; Butler, R. C.; Cuttaia, F.; de Rosa, A.; Finelli, F.; Franceschi, E.; Gruppuso, A.; Mandolesi, N.; Morgante, G.; Natoli, P.; Paoletti, D.; Sandri, M.; Terenzi, L.; Toffolatti, L.; Valenziano, L.; Villa, F.] IASF Bologna, INAF, Via Gobetti 101, I-40127 Bologna, Italy.
[Bersanelli, M.; Donzelli, S.; Maino, D.; Mennella, A.; Rossetti, M.; Tomasi, M.] IASF Milano, INAF, Via E Bassini 15, I-20133 Milan, Italy.
[Burigana, C.; Finelli, F.; Paoletti, D.] INFN, Sez Bologna, Via Irnerio 46, I-40126 Bologna, Italy.
[Melchiorri, A.; Pagano, L.] Univ Roma Sapienza, INFN, Sez Roma 1, Piazzale Aldo Moro 2, I-00185 Rome, Italy.
[Renzi, A.] Univ Roma Tor Vergata, INFN, Sez Roma 2, Via Ric Sci 1, I-00185 Rome, Italy.
[Gregorio, A.] Natl Inst Nucl Phys, INFN, Via Valerio 2, I-34127 Trieste, Italy.
[Desert, F. -X.] Univ Grenoble Alpes, IPAG, F-38000 Grenoble, France.
[Desert, F. -X.] IPAG, CNRS, F-38000 Grenoble, France.
[Mitra, S.] IUCAA, Post Bag 4,Ganeshkhind,Pune Univ Campus, Pune 411007, Maharashtra, India.
[Clements, D. L.; Ducout, A.; Jaffe, A. H.; Mortlock, D.] Imperial Coll London, Blackett Lab, Astrophys Grp, Prince Consort Rd, London SW7 2AZ, England.
[McGehee, P.; Pearson, T. J.; Rusholme, B.] CALTECH, Infrared Proc & Anal Ctr, Pasadena, CA 91125 USA.
[Benoit, A.] Univ Joseph Fourier Grenoble I, CNRS, Inst Neel, 25 Rue Martyrs, F-38000 Grenoble, France.
[Dole, H.] Inst Univ France, 103 Bd St Michel, F-75005 Paris, France.
[Aghanim, N.; Aumont, J.; Boulanger, F.; Chamballu, A.; Dole, H.; Douspis, M.; Ghosh, T.; Hurier, G.; Kunz, M.; Lagache, G.; Mangilli, A.; Miville-Deschenes, M. -A.; Pajot, F.; Puget, J. -L.; Remazeilles, M.] Univ Paris Sud 11, CNRS, Inst Astrophys Spatiale, UMR8617, Batiment 121, F-91898 Orsay, France.
[Benabed, K.; Benoit-Levy, A.; Bouchet, F. R.; Cardoso, J. -F.; Colombi, S.; Delouis, J. -M.; Ducout, A.; Elsner, F.; Hivon, E.; Moneti, A.; Prunet, S.; Sygnet, J. -F.; Wandelt, B. D.] Inst Astrophys Paris, CNRS, UMR7095, 98 Bis Blvd Arago, F-75014 Paris, France.
[Lesgourgues, J.] Rhein Westfal TH Aachen, Inst Theoret Teilchenphys & Kosmol, D-52056 Aachen, Germany.
[Challinor, A.; Efstathiou, G.; Gratton, S.; Harrison, D. L.; Migliaccio, M.; Sutton, D.] Univ Cambridge, Inst Astron, Madingley Rd, Cambridge CB3 0HA, England.
[Eriksen, H. K.; Gjerlow, E.; Hansen, F. K.; Lilje, P. B.] Univ Oslo, Inst Theoret Astrophys, N-0371 Oslo, Norway.
[Rebolo, R.; Rubino-Martin, J. A.] Inst Astrofis Canarias, C Via Lactea S-N, San Cristobal la Laguna 38205, Tenerife, Spain.
[Barreiro, R. B.; Bonavera, L.; Curto, A.; Diego, J. M.; Gonzalez-Nuevo, J.; Herranz, D.; Lopez-Caniego, M.; Martinez-Gonzalez, E.; Toffolatti, L.; Vielva, P.] Univ Cantabria, CSIC, Inst Fis Cantabria, Avda Los Castros S-N, Santander, Spain.
[Bartolo, N.; Liguori, M.; Matarrese, S.] Ist Nazl Fis Nucl, Sez Padova, Via Marzolo 8, I-35131 Padua, Italy.
[Bartlett, J. G.; Bock, J. J.; Colombo, L. P. L.; Crill, B. P.; Dore, O.; Gorski, K. M.; Hanson, D.; Hildebrandt, S. R.; Holmes, W. A.; Lawrence, C. R.; Mitra, S.; Pietrobon, D.; Prezeau, G.; Rocha, G.; Roudier, G.; Seiffert, M. D.; Wade, L. A.; Wehus, I. K.] CALTECH, Jet Prop Lab, 4800 Oak Grove Dr, Pasadena, CA USA.
[Bonaldi, A.; Davies, R. D.; Davis, R. J.; Dickinson, C.; Noviello, F.; Remazeilles, M.] Univ Manchester, Sch Phys & Astron, Jodrell Bank Ctr Astrophys, Alan Turing Bldg,Oxford Rd, Manchester M13 9PL, Lancs, England.
[Galli, S.] Univ Chicago, Kavli Inst Cosmol Phys, Chicago, IL 60637 USA.
[Ashdown, M.; Challinor, A.; Curto, A.; Gratton, S.; Harrison, D. L.; Lasenby, A.; Migliaccio, M.; Sutton, D.] Kavli Inst Cosmol Cambridge, Madingley Rd, Cambridge CB3 0HA, England.
[Stolyarov, V.] Kazan Fed Univ, 18 Kremlyovskaya St, Kazan 420008, Russia.
[Couchot, F.; Henrot-Versille, S.; Mangilli, A.; Perdereau, O.; Plaszczynski, S.; Tristram, M.] Univ Paris 11, LAL, CNRS IN2P3, F-91898 Orsay, France.
[Catalano, A.; Coulais, A.; Lamarre, J. -M.; Levrier, F.; Roudier, G.] Observ Paris, CNRS, LERMA, 61 Ave Observ, F-75000 Paris, France.
[Arnaud, M.; Chamballu, A.; Pratt, G. W.] Univ Paris Diderot, CEA Saclay, CNRS, Lab AIM IRFU,Serv Astrophys,CEA,DSM, Bat 709, F-91191 Gif Sur Yvette, France.
[Cardoso, J. -F.] CNRS, UMR 5141, Lab Traitement & Commun Informat, 46 Rue Barrault, F-75634 Paris 13, France.
[Cardoso, J. -F.] Telecom ParisTech, 46 Rue Barrault, F-75634 Paris 13, France.
[Catalano, A.; Combet, C.; Macias-Perez, J. F.; Perotto, L.; Renault, C.; Santos, D.] Univ Grenoble Alpes, CNRS IN2P3, Lab Phys Subat & Cosmol, 53 Rue Martyrs, F-38026 Grenoble, France.
[Van Tent, B.] Univ Paris Sud 11, Lab Phys Theor, Batiment 210, F-91405 Orsay, France.
[Van Tent, B.] CNRS, Batiment 210, F-91405 Orsay, France.
[Kisner, T. S.] Lawrence Berkeley Natl Lab, Berkeley, CA 94720 USA.
[Novikov, D.; Novikov, I.] Russian Acad Sci, Astro Space Ctr, Lebedev Phys Inst, 84-32 Profsoyuznaya St,GSP-7, Moscow 117997, Russia.
[Dolag, K.; Ensslin, T. A.; Hernandez-Monteagudo, C.; Hovest, W.; Knoche, J.; Rachen, J. P.; Reinecke, M.] Max Planck Inst Astrophys, Karl Schwarzschild Str 1, D-85741 Garching, Germany.
[Hanson, D.] McGill Univ, McGill Phys, Ernest Rutherford Phys Bldg,3600 Rue Univ, Montreal, PQ H3A 2T8, Canada.
[Murphy, J. A.] Natl Univ Ireland, Dept Expt Phys, Maynooth, Co Kildare, Ireland.
[Bielewicz, P.] Nicolaus Copernicus Astron Ctr, Bartycka 18, PL-00716 Warsaw, Poland.
[Christensen, P. R.; Frejsel, A.; Naselsky, P.; Novikov, I.] Niels Bohr Inst, Blegdamsvej 17, DK-1165 Copenhagen, Denmark.
[Baccigalupi, C.; Bielewicz, P.; Danese, L.; de Zotti, G.; Paci, F.; Perrotta, F.] SISSA, Astrophys Sect, Via Bonomea 265, I-34136 Trieste, Italy.
[Ade, P. A. R.; Munshi, D.; Spencer, L. D.; Sudiwala, R.] Cardiff Univ, Sch Phys & Astron, Queens Bldg, Cardiff CF24 3AA, S Glam, Wales.
[Moss, A.] Univ Nottingham, Sch Phys & Astron, Nottingham NG7 2RD, England.
[Bouchet, F. R.] UPMC, Sorbonne Univ, UMR7095, Inst Astrophys Paris, 98 Bis Blvd Arago, F-75014 Paris, France.
[Borrill, J.] Univ Calif Berkeley, Space Sci Lab, Berkeley, CA 94720 USA.
[Stolyarov, V.] Russian Acad Sci, Special Astrophys Observ, Karachai Cherkessian Rep 369167, Russia.
[Calabrese, E.; Welikala, N.] Univ Oxford, Subdept Astrophys, Keble Rd, Oxford OX1 3RH, England.
[Lesgourgues, J.] CERN, Div Theory, PH TH, CH-1211 Geneva 23, Switzerland.
[Benabed, K.; Benoit-Levy, A.; Colombi, S.; Delouis, J. -M.; Elsner, F.; Hivon, E.; Prunet, S.; Wandelt, B. D.] UPMC Univ Paris 06, UMR7095, 98 Bis Blvd Arago, F-75014 Paris, France.
[Banday, A. J.; Bernard, J. -P.; Forni, O.; Giard, M.; Jaffe, T. R.; Montier, L.; Pointecouteau, E.; Ristorcelli, I.] Univ Toulouse, UPS OMP, IRAP, F-31028 Toulouse 4, France.
[Dolag, K.] Ludwig Maximilian Univ Munich, Univ Observ, Scheinerstr 1, D-81679 Munich, Germany.
[Battaner, E.] Univ Granada, Fac Ciencias, Dept Fis Teor & Cosmos, Granada 18010, Spain.
[Battaner, E.] Univ Granada, Inst Carlos I Fis Teor & Computac, E-18071 Granada, Spain.
[Gorski, K. M.] Univ Warsaw Observ, Aleje Ujazdowskie 4, PL-00478 Warsaw, Poland.
RP Borrill, J (reprint author), Lawrence Berkeley Natl Lab, Computat Cosmol Ctr, Berkeley, CA 92093 USA.; Borrill, J (reprint author), Univ Calif Berkeley, Space Sci Lab, Berkeley, CA 94720 USA.
EM jdborrill@lbl.gov
RI bonavera, laura/E-9368-2017; Gonzalez-Nuevo, Joaquin/I-3562-2014;
Herranz, Diego/K-9143-2014; Colombo, Loris/J-2415-2016; Barreiro, Rita
Belen/N-5442-2014
OI Toffolatti, Luigi/0000-0003-2645-7386; Lilje, Per/0000-0003-4324-7794;
Nati, Federico/0000-0002-8307-5088; Pierpaoli,
Elena/0000-0002-7957-8993; Juvela, Mika/0000-0002-5809-4834; bonavera,
laura/0000-0001-8039-3876; Gonzalez-Nuevo, Joaquin/0000-0003-1354-6822;
Herranz, Diego/0000-0003-4540-1417; Colombo, Loris/0000-0003-4572-7732;
Valiviita, Jussi/0000-0001-6225-3693; Kurki-Suonio,
Hannu/0000-0002-4618-3063; Zacchei, Andrea/0000-0003-0396-1192;
Stolyarov, Vladislav/0000-0001-8151-828X; Paoletti,
Daniela/0000-0003-4761-6147; TERENZI, LUCA/0000-0001-9915-6379;
Barreiro, Rita Belen/0000-0002-6139-4272
FU ESA; CNES (France); CNRS/INSU-IN2P3-INP (France); ASI (Italy); CNR
(Italy); INAF (Italy); NASA (USA); DoE (USA); STFC (UK); UKSA (UK); CSIC
(Spain); MINECO (Spain); JA (Spain); RES (Spain); Tekes (Finland); AoF
(Finland); CSC (Finland); DLR (Germany); MPG (Germany); CSA (Canada);
DTU Space (Denmark); SER/SSO (Switzerland); RCN (Norway); SFI (Ireland);
FCT/MCTES (Portugal); ERC (EU); PRACE (EU)
FX The Planck Collaboration acknowledges the support of: ESA; CNES and
CNRS/INSU-IN2P3-INP (France); ASI, CNR, and INAF (Italy); NASA and DoE
(USA); STFC and UKSA (UK); CSIC, MINECO, JA, and RES (Spain); Tekes,
AoF, and CSC (Finland); DLR and MPG (Germany); CSA (Canada); DTU Space
(Denmark); SER/SSO (Switzerland); RCN (Norway); SFI (Ireland); FCT/MCTES
(Portugal); ERC and PRACE (EU). A description of the Planck
Collaboration and a list of its members, indicating which technical or
scientific activities they have been involved in, can be found at
http://www.cosmos.esa.int/web/planck/planck-collaboration. Particular
thanks are due to the extraordinary NERSC staff, who have supported the
Planck mission for over a decade and who facilitated the production and
distribution of FFP8 in numerous ways.
NR 105
TC 0
Z9 0
U1 0
U2 0
PU EDP SCIENCES S A
PI LES ULIS CEDEX A
PA 17, AVE DU HOGGAR, PA COURTABOEUF, BP 112, F-91944 LES ULIS CEDEX A,
FRANCE
SN 1432-0746
J9 ASTRON ASTROPHYS
JI Astron. Astrophys.
PD OCT
PY 2016
VL 594
AR A12
DI 10.1051/0004-6361/201527103
PG 28
WC Astronomy & Astrophysics
SC Astronomy & Astrophysics
GA DZ4MG
UT WOS:000385832200031
ER
PT J
AU Ade, PAR
Aumont, J
Baccigalupi, C
Banday, AJ
Barreiro, RB
Bartolo, N
Basak, S
Battaglia, P
Battaner, E
Benabed, K
Benoit-Levy, A
Bernard, JP
Bersanelli, M
Bielewicz, P
Bonaldi, A
Bonavera, L
Bond, JR
Borrill, J
Burigana, C
Butler, RC
Calabrese, E
Catalano, A
Christensen, PR
Colombo, LPL
Cruz, M
Curto, A
Cuttaia, F
Danese, L
Davies, RD
Davis, RJ
de Bernardis, P
de Rosa, A
de Zotti, G
Delabrouille, J
Dickinson, C
Diego, JM
Dore, O
Ducout, A
Dupac, X
Elsner, F
Ensslin, TA
Eriksen, HK
Finelli, F
Frailis, M
Franceschet, C
Franceschi, E
Galeotta, S
Galli, S
Ganga, K
Ghosh, T
Giard, M
Giraud-Heraud, Y
Gjerlow, E
Gonzalez-Nuevo, J
Gorski, KM
Gregorio, A
Gruppuso, A
Hansen, FK
Harrison, DL
Hernandez-Monteagudo, C
Herranz, D
Hildebrandt, SR
Hivon, E
Hobson, M
Hornstrup, A
Hovest, W
Huffenberger, KM
Hurier, G
Jaffe, AH
Jaffe, TR
Keihanen, E
Keskitalo, R
Kiiveri, K
Kisner, TS
Knoche, J
Krachmalnicoff, N
Kunz, M
Kurki-Suonio, H
Lagache, G
Lamarre, JM
Lasenby, A
Lattanzi, M
Lawrence, CR
Leahy, JP
Leonardi, R
Levrier, F
Liguori, M
Lilje, PB
Linden-Vornle, M
Lindholm, V
Lopez-Caniego, M
Lubin, PM
Macias-Perez, JF
Maffei, B
Maggio, G
Maino, D
Mandolesi, N
Mangilli, A
Maris, M
Martin, PG
Martinez-Gonzalez, E
Masi, S
Matarrese, S
Meinhold, PR
Mennella, A
Migliaccio, M
Mitra, S
Montier, L
Morgante, G
Mortlock, D
Munshi, D
Murphy, JA
Nati, F
Natoli, P
Noviello, F
Paci, F
Pagano, L
Pajot, F
Paoletti, D
Partridge, B
Pasian, F
Pearson, TJ
Perdereau, O
Pettorino, V
Piacentini, F
Pointecouteau, E
Polenta, G
Pratt, GW
Puget, JL
Rachen, JP
Reinecke, M
Remazeilles, M
Renzi, A
Ristorcelli, I
Rocha, G
Rosset, C
Rossetti, M
Roudier, G
Rubino-Martin, JA
Rusholme, B
Sandri, M
Santos, D
Savelainen, M
Scott, D
Stolyarov, V
Stompor, R
Suur-Uski, AS
Sygnet, JF
Tauber, JA
Tavagnacco, D
Terenzi, L
Toffolatti, L
Tomasi, M
Tristram, M
Tucci, M
Umana, G
Valenziano, L
Valiviita, J
Van Tent, B
Vassallo, T
Vielva, P
Villa, F
Wade, LA
Wandelt, BD
Watson, R
Wehus, IK
Yvon, D
Zacchei, A
Zibin, JP
Zonca, A
AF Ade, P. A. R.
Aumont, J.
Baccigalupi, C.
Banday, A. J.
Barreiro, R. B.
Bartolo, N.
Basak, S.
Battaglia, P.
Battaner, E.
Benabed, K.
Benoit-Levy, A.
Bernard, J. -P.
Bersanelli, M.
Bielewicz, P.
Bonaldi, A.
Bonavera, L.
Bond, J. R.
Borrill, J.
Burigana, C.
Butler, R. C.
Calabrese, E.
Catalano, A.
Christensen, P. R.
Colombo, L. P. L.
Cruz, M.
Curto, A.
Cuttaia, F.
Danese, L.
Davies, R. D.
Davis, R. J.
de Bernardis, P.
de Rosa, A.
de Zotti, G.
Delabrouille, J.
Dickinson, C.
Diego, J. M.
Dore, O.
Ducout, A.
Dupac, X.
Elsner, F.
Ensslin, T. A.
Eriksen, H. K.
Finelli, F.
Frailis, M.
Franceschet, C.
Franceschi, E.
Galeotta, S.
Galli, S.
Ganga, K.
Ghosh, T.
Giard, M.
Giraud-Heraud, Y.
Gjerlow, E.
Gonzalez-Nuevo, J.
Gorski, K. M.
Gregorio, A.
Gruppuso, A.
Hansen, F. K.
Harrison, D. L.
Hernandez-Monteagudo, C.
Herranz, D.
Hildebrandt, S. R.
Hivon, E.
Hobson, M.
Hornstrup, A.
Hovest, W.
Huffenberger, K. M.
Hurier, G.
Jaffe, A. H.
Jaffe, T. R.
Keihanen, E.
Keskitalo, R.
Kiiveri, K.
Kisner, T. S.
Knoche, J.
Krachmalnicoff, N.
Kunz, M.
Kurki-Suonio, H.
Lagache, G.
Lamarre, J. -M.
Lasenby, A.
Lattanzi, M.
Lawrence, C. R.
Leahy, J. P.
Leonardi, R.
Levrier, F.
Liguori, M.
Lilje, P. B.
Linden-Vornle, M.
Lindholm, V.
Lopez-Caniego, M.
Lubin, P. M.
Macias-Perez, J. F.
Maffei, B.
Maggio, G.
Maino, D.
Mandolesi, N.
Mangilli, A.
Maris, M.
Martin, P. G.
Martinez-Gonzalez, E.
Masi, S.
Matarrese, S.
Meinhold, P. R.
Mennella, A.
Migliaccio, M.
Mitra, S.
Montier, L.
Morgante, G.
Mortlock, D.
Munshi, D.
Murphy, J. A.
Nati, F.
Natoli, P.
Noviello, F.
Paci, F.
Pagano, L.
Pajot, F.
Paoletti, D.
Partridge, B.
Pasian, F.
Pearson, T. J.
Perdereau, O.
Pettorino, V.
Piacentini, F.
Pointecouteau, E.
Polenta, G.
Pratt, G. W.
Puget, J. -L.
Rachen, J. P.
Reinecke, M.
Remazeilles, M.
Renzi, A.
Ristorcelli, I.
Rocha, G.
Rosset, C.
Rossetti, M.
Roudier, G.
Rubino-Martin, J. A.
Rusholme, B.
Sandri, M.
Santos, D.
Savelainen, M.
Scott, D.
Stolyarov, V.
Stompor, R.
Suur-Uski, A. -S.
Sygnet, J. -F.
Tauber, J. A.
Tavagnacco, D.
Terenzi, L.
Toffolatti, L.
Tomasi, M.
Tristram, M.
Tucci, M.
Umana, G.
Valenziano, L.
Valiviita, J.
Van Tent, B.
Vassallo, T.
Vielva, P.
Villa, F.
Wade, L. A.
Wandelt, B. D.
Watson, R.
Wehus, I. K.
Yvon, D.
Zacchei, A.
Zibin, J. P.
Zonca, A.
CA Planck Collaboration
TI Planck 2015 results III. LFI systematic uncertainties
SO ASTRONOMY & ASTROPHYSICS
LA English
DT Article
DE cosmic background radiation; cosmology: observations; space vehicles:
instruments; methods: data analysis
ID LOW-FREQUENCY INSTRUMENT; PRIMORDIAL NON-GAUSSIANITY; STRAYLIGHT
CONTAMINATION; ANGULAR RESOLUTION; TRADE-OFF; SKY MAPS; POLARIZATION;
BISPECTRUM; MISSION
AB We present the current accounting of systematic effect uncertainties for the Low Frequency Instrument (LFI) that are relevant to the 2015 release of the Planck cosmological results, showing the robustness and consistency of our data set, especially for polarization analysis. We use two complementary approaches: (i) simulations based on measured data and physical models of the known systematic effects; and (ii) analysis of difference maps containing the same sky signal ("null-maps"). The LFI temperature data are limited by instrumental noise. At large angular scales the systematic effects are below the cosmic microwave background (CMB) temperature power spectrum by several orders of magnitude. In polarization the systematic uncertainties are dominated by calibration uncertainties and compete with the CMB E-modes in the multipole range 10-20. Based on our model of all known systematic effects, we show that these effects introduce a slight bias of around 0.2 sigma on the reionization optical depth derived from the 70 GHz EE spectrum using the 30 and 353 GHz channels as foreground templates. At 30 GHz the systematic effects are smaller than the Galactic foreground at all scales in temperature and polarization, which allows us to consider this channel as a reliable template of synchrotron emission. We assess the residual uncertainties due to LFI effects on CMB maps and power spectra after component separation and show that these effects are smaller than the CMB amplitude at all scales. We also assess the impact on non-Gaussianity studies and find it to be negligible. Some residuals still appear in null maps from particular sky survey pairs, particularly at 30 GHz, suggesting possible straylight contamination due to an imperfect knowledge of the beam far sidelobes.
C1 [Delabrouille, J.; Ganga, K.; Giraud-Heraud, Y.; Remazeilles, M.; Rosset, C.; Roudier, G.; Stompor, R.] Univ Paris Diderot, CNRS IN2P3, APC AstroParticule & Cosmol, CEA Irfu,Observ Paris,Sorbonne Paris Cite, 10 Rue Alice Domon & Leonie Duquet, F-75205 Paris 13, France.
[Kunz, M.] African Inst Math Sci, 6-8 Melrose Rd, ZA-7945 Cape Town, South Africa.
[Natoli, P.; Polenta, G.] Agenzia Spaziale Italiana Sci Data Ctr, Via Politecn Snc, I-00133 Rome, Italy.
[Lagache, G.] Aix Marseille Univ, CNRS, LAM Lab Astrophys Marseille, UMR 7326, F-13388 Marseille, France.
[Curto, A.; Hobson, M.; Lasenby, A.; Stolyarov, V.] Univ Cambridge, Cavendish Lab, Astrophys Grp, JJ Thomson Ave, Cambridge CB3 0HE, England.
[Leonardi, R.] CGEE, SCS Qd 9,Lote C,Tone C,4 Andar, BR-70308200 Brasilia, DF, Brazil.
[Bond, J. R.; Martin, P. G.] Univ Toronto, CITA, 60 St George St, Toronto, ON M5S 3H8, Canada.
[Banday, A. J.; Bernard, J. -P.; Bielewicz, P.; Giard, M.; Jaffe, T. R.; Montier, L.; Pointecouteau, E.; Ristorcelli, I.] IRAP, CNRS, 9 Av Colonel Roche,BP 44346, F-31028 Toulouse 4, France.
[Dore, O.; Hildebrandt, S. R.; Pearson, T. J.; Rocha, G.] CALTECH, Pasadena, CA 91125 USA.
[Hernandez-Monteagudo, C.] Ctr Estudios Fis Cosmos Aragon CEFCA, Plaza San Juan 1,Planta 2, Teruel 44001, Spain.
[Borrill, J.; Keskitalo, R.] Lawrence Berkeley Natl Lab, Computat Cosmol Ctr, Berkeley, CA 94720 USA.
[Yvon, D.] CEA Saclay, DSM Irfu SPP, F-91191 Gif Sur Yvette, France.
[Hornstrup, A.; Linden-Vornle, M.] Tech Univ Denmark, Natl Space Inst, DTU Space, Elektrovej 327, DK-2800 Lyngby, Denmark.
[Kunz, M.; Tucci, M.] Univ Geneva, Dept Phys Theor, 24 Quai E Ansermet, CH-1211 Geneva 4, Switzerland.
[Rubino-Martin, J. A.] Univ La Laguna ULL, Dept Astrofis, San Cristobal la Laguna 38206, Tenerife, Spain.
[Gonzalez-Nuevo, J.; Toffolatti, L.] Univ Oviedo, Dept Fis, Avda Calvo Sotelo S-N, Oviedo 33003, Spain.
[Cruz, M.] Univ Cantabria, Dept Matemat Estadist & Computac, Avda Los Castros S-N, Santander 39005, Spain.
[Rachen, J. P.] Radboud Univ Nijmegen, IMAPP, Dept Astrophys, POB 9010, NL-6500 GL Nijmegen, Netherlands.
[Scott, D.; Zibin, J. P.] Univ British Columbia, Dept Phys & Astron, 6224 Agr Rd, Vancouver, BC, Canada.
[Colombo, L. P. L.] Univ Southern Calif, Dana & David Dornsife Coll Letter Arts & Sci, Dept Phys & Astron, Los Angeles, CA 90089 USA.
[Benoit-Levy, A.; Elsner, F.] UCL, Dept Phys & Astron, London WC1E 6BT, England.
[Huffenberger, K. M.] Florida State Univ, Dept Phys, Keen Phys Bldg,77 Chieftan Way, Tallahassee, FL 32306 USA.
[Keihanen, E.; Kiiveri, K.; Kurki-Suonio, H.; Lindholm, V.; Savelainen, M.; Suur-Uski, A. -S.; Valiviita, J.] Univ Helsinki, Dept Phys, Gustaf Hallstromin Katu 2a, Helsinki 00100, Finland.
[Nati, F.] Princeton Univ, Dept Phys, Princeton, NJ 08544 USA.
[Lubin, P. M.; Meinhold, P. R.; Zonca, A.] Univ Calif Santa Barbara, Dept Phys, Santa Barbara, CA 93106 USA.
[Wandelt, B. D.] Univ Illinois, Dept Phys, 1110 West Green St, Urbana, IL USA.
[Bartolo, N.; Liguori, M.; Matarrese, S.] Univ Padua, Dipartimento Fis & Astron G Galilei, Via Marzolo 8, I-35131 Padua, Italy.
[Burigana, C.; Lattanzi, M.; Mandolesi, N.; Natoli, P.] Univ Ferrara, Dipartimento Fis & Sci Terra, Via Saragat 1, I-44122 Ferrara, Italy.
[Battaglia, P.; de Bernardis, P.; Masi, S.; Pagano, L.; Piacentini, F.] Univ La Sapienza, Dipartimento Fis, Ple A Moro 2, Rome, Italy.
[Bersanelli, M.; Franceschet, C.; Krachmalnicoff, N.; Maino, D.; Mennella, A.; Rossetti, M.; Tomasi, M.] Univ Milan, Dipartimento Fis, Via Celoria 16, Milan, Italy.
[Battaglia, P.; Gregorio, A.; Tavagnacco, D.] Univ Trieste, Dipartimento Fis, Via A Valerio 2, I-24128 Trieste, Italy.
[Renzi, A.] Univ Roma Tor Vergata, Dipartimento Matemat, Via Ric Sci 1, Rome, Italy.
[Christensen, P. R.] Niels Bohr Inst, Discovery Ctr, Blegdamsvej 17, DK-2100 Copenhagen, Denmark.
[Dupac, X.; Lopez-Caniego, M.] European Space Agcy ESAC, Planck Sci Off, Camino Bajo del Castillo S-N, Madrid 28692, Spain.
[Tauber, J. A.] European Space Agcy ESTEC, Keplerlaan 1, NL-2201 AZ Noordwijk, Netherlands.
[Matarrese, S.] INFN, Gran Sasso Sci Inst, Viale F Crispi 7, I-67100 Laquila, Italy.
[Pettorino, V.] HGSFP, Philosophenweg 16, D-69120 Heidelberg, Germany.
[Pettorino, V.] Heidelberg Univ, Dept Theoret Phys, Philosophenweg 16, D-69120 Heidelberg, Germany.
[Partridge, B.] Haverford Coll, Dept Astron, 370 Lancaster Ave, Haverford, PA USA.
[Kiiveri, K.; Kurki-Suonio, H.; Lindholm, V.; Savelainen, M.; Suur-Uski, A. -S.; Valiviita, J.] Univ Helsinki, Helsinki Inst Phys, Gustaf Hallstromin Katu 2, Helsinki 00100, Finland.
[Umana, G.] INAF, Osservatorio Astrofis Catania, Via S Sofia 78, Catania, Italy.
[de Zotti, G.] INAF, Osservatorio Astron Padova, Vicolo Osservatorio 5, I-35122 Padua, Italy.
[Polenta, G.] INAF, Osservatorio Astron Roma, Via Frascati 33, I-00078 Monte Porzio Catone, Italy.
[Frailis, M.; Galeotta, S.; Gregorio, A.; Maggio, G.; Maris, M.; Pasian, F.; Tavagnacco, D.; Vassallo, T.; Zacchei, A.] INAF, Osservatorio Astron Trieste, Via GB Tiepolo 11, I-34131 Trieste, Italy.
[Burigana, C.; Butler, R. C.; Cuttaia, F.; de Rosa, A.; Finelli, F.; Franceschi, E.; Gruppuso, A.; Mandolesi, N.; Morgante, G.; Natoli, P.; Paoletti, D.; Sandri, M.; Terenzi, L.; Toffolatti, L.; Valenziano, L.; Villa, F.] INAF, IASF Bologna, Via Gobetti 101, I-40127 Bologna, Italy.
[Bersanelli, M.; Maino, D.; Mennella, A.; Rossetti, M.; Tomasi, M.] INAF, IASF Milano, Via E Bassini 15, I-20133 Milan, Italy.
[Burigana, C.; Finelli, F.; Paoletti, D.] INFN, Sez Bologna, Via Irnerio 46, I-40126 Bologna, Italy.
[Pagano, L.] Univ Roma Sapienza, INFN, Sez Roma 1, Ple Aldo Moro 2, I-00185 Rome, Italy.
[Renzi, A.] Univ Roma Tor Vergata, INFN, Sez Roma 2, Via Ric Sci 1, Rome, Italy.
[Gregorio, A.] INFN, Natl Inst Nucl Phys, Via Valerio 2, I-34127 Trieste, Italy.
[Mitra, S.] IUCAA, Post Bag 4,Pune Univ Campus, Pune 411007, Maharashtra, India.
[Ducout, A.; Jaffe, A. H.; Mortlock, D.] Imperial Coll London, Blackett Lab, Astrophys Grp, Prince Consort Rd, London SW7 2AZ, England.
[Pearson, T. J.; Rusholme, B.] CALTECH, Infrared Proc & Anal Ctr, Pasadena, CA 91125 USA.
[Aumont, J.; Ghosh, T.; Hurier, G.; Kunz, M.; Lagache, G.; Mangilli, A.; Pajot, F.; Puget, J. -L.; Remazeilles, M.] Univ Paris Saclay, Univ Paris Sud, CNRS, Inst Astrophys Spatiale, Bat 121, F-91405 Orsay, France.
[Benabed, K.; Benoit-Levy, A.; Ducout, A.; Elsner, F.; Hivon, E.; Sygnet, J. -F.; Wandelt, B. D.] Inst Astrophys Paris, CNRS, UMR 7095, 98bis Blvd Arago, F-75014 Paris, France.
[Harrison, D. L.; Migliaccio, M.] Univ Cambridge, Inst Astron, Madingley Rd, Cambridge CB3 0HA, England.
[Eriksen, H. K.; Gjerlow, E.; Hansen, F. K.; Lilje, P. B.; Wehus, I. K.] Univ Oslo, Inst Theoret Astrophys, N-0371 Oslo, Norway.
[Rubino-Martin, J. A.] Inst Astrofis Canarias, C Via Lactea S-N, San Cristobal la Laguna 38205, Tenerife, Spain.
[Barreiro, R. B.; Bonavera, L.; Curto, A.; Diego, J. M.; Gonzalez-Nuevo, J.; Herranz, D.; Lopez-Caniego, M.; Martinez-Gonzalez, E.; Toffolatti, L.; Vielva, P.] Univ Cantabria, CSIC, Inst Fis Cantabria, Avda Los Castros S-N, E-39005 Santander, Spain.
[Bartolo, N.; Liguori, M.; Matarrese, S.] Ist Nazl Fis Nucl, Sez Padova, Via Marzolo 8, I-35131 Padua, Italy.
[Colombo, L. P. L.; Dore, O.; Gorski, K. M.; Hildebrandt, S. R.; Lawrence, C. R.; Mitra, S.; Rocha, G.; Roudier, G.; Wade, L. A.; Wehus, I. K.] CALTECH, Jet Prop Lab, 4800 Oak Grove Dr, Pasadena, CA USA.
[Bonaldi, A.; Davies, R. D.; Davis, R. J.; Dickinson, C.; Leahy, J. P.; Maffei, B.; Noviello, F.; Remazeilles, M.; Watson, R.] Univ Manchester, Sch Phys & Astron, Jodrell Bank Ctr Astrophys, Alan Turing Bldg,Oxford Rd, Manchester M13 9PL, Lancs, England.
[Galli, S.] Univ Chicago, Kavli Inst Cosmol Phys, Chicago, IL 60637 USA.
[Curto, A.; Harrison, D. L.; Lasenby, A.; Migliaccio, M.] Kavli Inst Cosmol Cambridge, Madingley Rd, Cambridge CB3 0HA, England.
[Stolyarov, V.] Kazan Fed Univ, 18 Kremlyovskaya St, Kazan 420008, Russia.
[Mangilli, A.; Perdereau, O.; Tristram, M.] Univ Paris 11, CNRS, LAL, IN2P3, Orsay, France.
[Catalano, A.; Lamarre, J. -M.; Levrier, F.; Roudier, G.] LERMA, CNRS, Observ Paris, 61 Ave Observ, F-75104 Paris, France.
[Pratt, G. W.] Univ Paris Diderot, CEA Saclay, CNRS, CEA DSM,Lab AIM,IRFU Serv Astrophys, Bat 709, F-91191 Gif Sur Yvette, France.
[Catalano, A.; Macias-Perez, J. F.; Santos, D.] Univ Grenoble Alpes, IN2P3, CNRS, Lab Phys Subat & Cosmol, 53 Rue Martyrs, F-38026 Grenoble, France.
[Van Tent, B.] Univ Paris Sud 11, Lab Phys Theor, Batiment 210, F-91405 Orsay, France.
[Van Tent, B.] CNRS, Batiment 210, F-91405 Orsay, France.
[Kisner, T. S.] Lawrence Berkeley Natl Lab, Berkeley, CA 94720 USA.
[Ensslin, T. A.; Hernandez-Monteagudo, C.; Hovest, W.; Knoche, J.; Rachen, J. P.; Reinecke, M.] Max Planck Inst Astrophys, Karl Schwarzschild Str 1, D-85741 Garching, Germany.
[Murphy, J. A.] Natl Univ Ireland, Dept Expt Phys, Maynooth, Co Kildare, Ireland.
[Bielewicz, P.] Nicolaus Copernicus Astron Ctr, Bartycka 18, PL-00716 Warsaw, Poland.
[Christensen, P. R.] Niels Bohr Inst, Blegdamsvej 17, Copenhagen, Denmark.
[Baccigalupi, C.; Basak, S.; Bielewicz, P.; Danese, L.; de Zotti, G.; Paci, F.] SISSA, Astrophys Sect, Via Bonomea 265, I-34136 Trieste, Italy.
[Terenzi, L.] Univ E Campus, SMARTEST Res Ctr, Via Isimbardi 10, I-22060 Novedrate, CO, Italy.
[Ade, P. A. R.; Munshi, D.] Cardiff Univ, Sch Phys & Astron, Queens Bldg, Cardiff CF24 3AA, S Glam, Wales.
[Borrill, J.] Univ Calif Berkeley, Space Sci Lab, Berkeley, CA 94720 USA.
[Stolyarov, V.] Russian Acad Sci, Special Astrophys Observ, Karachai Cherkessian Rep 369167, Russia.
[Calabrese, E.] Univ Oxford, Subdept Astrophys, Keble Rd, Oxford OX1 3RH, England.
[Benabed, K.; Benoit-Levy, A.; Elsner, F.; Hivon, E.; Wandelt, B. D.] UPMC Univ Paris 06, UMR 7095, 98bis Blvd Arago, F-75014 Paris, France.
[Banday, A. J.; Benoit-Levy, A.; Bernard, J. -P.; Giard, M.; Montier, L.; Pointecouteau, E.; Ristorcelli, I.] Univ Toulouse, UPS OMP, IRAP, F-31028 Toulouse 4, France.
[Battaner, E.] Univ Granada, Fac Ciencias, Dept Fis Teor & Cosmos, Granada 18010, Spain.
[Battaner, E.] Univ Granada, Inst Carlos I Fis Teor & Computac, Granada 18010, Spain.
[Gorski, K. M.] Univ Warsaw Observ, Aleje Ujazdowskie 4, PL-00478 Warsaw, Poland.
RP Ade, PAR (reprint author), Cardiff Univ, Sch Phys & Astron, Queens Bldg, Cardiff CF24 3AA, S Glam, Wales.
RI Barreiro, Rita Belen/N-5442-2014; bonavera, laura/E-9368-2017;
Gonzalez-Nuevo, Joaquin/I-3562-2014; Herranz, Diego/K-9143-2014;
Colombo, Loris/J-2415-2016;
OI Hurier, Guillaume/0000-0002-1215-0706; Barreiro, Rita
Belen/0000-0002-6139-4272; bonavera, laura/0000-0001-8039-3876;
Gonzalez-Nuevo, Joaquin/0000-0003-1354-6822; Herranz,
Diego/0000-0003-4540-1417; Colombo, Loris/0000-0003-4572-7732;
Valiviita, Jussi/0000-0001-6225-3693; Kurki-Suonio,
Hannu/0000-0002-4618-3063; Zacchei, Andrea/0000-0003-0396-1192;
Stolyarov, Vladislav/0000-0001-8151-828X; TERENZI,
LUCA/0000-0001-9915-6379; Piacentini, Francesco/0000-0002-5444-9327;
Toffolatti, Luigi/0000-0003-2645-7386; Paoletti,
Daniela/0000-0003-4761-6147; Nati, Federico/0000-0002-8307-5088
FU ESA; CNES (France); CNRS/INSU-IN2P3-INP (France); ASI (Italy); CNR
(Italy); INAF (Italy); NASA (USA); DoE (USA); STFC (UK); UKSA (UK); CSIC
(Spain); MINECO (Spain); JA (Spain); RES (Spain); Tekes (Finland); AoF
(Finland); CSC (Finland); DLR (Germany); MPG (Germany); CSA (Canada);
DTU Space (Denmark); SER/SSO (Switzerland); RCN (Norway); SFI (Ireland);
FCT/MCTES (Portugal); ERC (EU); PRACE (EU)
FX The Planck Collaboration acknowledges the support of: ESA; CNES, and
CNRS/INSU-IN2P3-INP (France); ASI, CNR, and INAF (Italy); NASA and DoE
(USA); STFC and UKSA (UK); CSIC, MINECO, JA, and RES (Spain); Tekes,
AoF, and CSC (Finland); DLR and MPG (Germany); CSA (Canada); DTU Space
(Denmark); SER/SSO (Switzerland); RCN (Norway); SFI (Ireland); FCT/MCTES
(Portugal); ERC and PRACE (EU). A description of the Planck
Collaboration and a list of its members, indicating which technical or
scientific activities they have been involved in, can be found at
http://www.cosmos.esa.int/web/planck/planck_collaboration. Some of the
results in this paper have been derived using the HEALPix package.
NR 59
TC 0
Z9 0
U1 0
U2 0
PU EDP SCIENCES S A
PI LES ULIS CEDEX A
PA 17, AVE DU HOGGAR, PA COURTABOEUF, BP 112, F-91944 LES ULIS CEDEX A,
FRANCE
SN 1432-0746
J9 ASTRON ASTROPHYS
JI Astron. Astrophys.
PD OCT
PY 2016
VL 594
AR A3
DI 10.1051/0004-6361/201526998
PG 32
WC Astronomy & Astrophysics
SC Astronomy & Astrophysics
GA DZ4MG
UT WOS:000385832200027
ER
PT J
AU Ade, PAR
Aghanim, N
Argueso, F
Arnaud, M
Ashdown, M
Aumont, J
Baccigalupi, C
Banday, AJ
Barreiro, RB
Bartolo, N
Battaner, E
Beichman, C
Benabed, K
Benoit, A
Benoit-Levy, A
Bernard, JP
Bersanelli, M
Bielewicz, P
Bock, JJ
Bohringer, H
Bonaldi, A
Bonavera, L
Bond, JR
Borrill, J
Bouchet, FR
Boulanger, F
Bucher, M
Burigana, C
Butler, RC
Calabrese, E
Cardoso, JF
Carvalho, P
Catalano, A
Challinor, A
Chamballu, A
Chary, RR
Chiang, HC
Christensen, PR
Clemens, M
Clements, DL
Colombi, S
Colombo, LPL
Combet, C
Couchot, F
Coulais, A
Crill, BP
Curto, A
Cuttaia, F
Danese, L
Davies, RD
Davis, RJ
de Bernardis, P
de Rosa, A
de Zotti, G
Delabrouille, J
Desert, FX
Dickinson, C
Diego, JM
Dole, H
Donzelli, S
Dore, O
Douspis, M
Ducout, A
Dupac, X
Efstathiou, G
Elsner, F
Ensslin, TA
Eriksen, HK
Falgarone, E
Fergusson, J
Finelli, F
Forni, O
Frailis, M
Fraisse, AA
Franceschi, E
Frejsel, A
Galeotta, S
Galli, S
Ganga, K
Giard, M
Giraud-Heraud, Y
Gjerlow, E
Gonzalez-Nuevo, J
Gorski, KM
Gratton, S
Gregorio, A
Gruppuso, A
Gudmundsson, JE
Hansen, FK
Hanson, D
Harrison, DL
Helou, G
Henrot-Versille, S
Hernandez-Monteagudo, C
Herranz, D
Hildebrandt, SR
Hivon, E
Hobson, M
Holmes, WA
Hornstrup, A
Hovest, W
Huffenberger, KM
Hurier, G
Jaffe, AH
Jaffe, TR
Jones, WC
Juvela, M
Keihanen, E
Keskitalo, R
Kisner, TS
Kneissl, R
Knoche, J
Kunz, M
Kurki-Suonio, H
Lagache, G
Lahteenmaki, A
Lamarre, JM
Lasenby, A
Lattanzi, M
Lawrence, CR
Leahy, JP
Leonardi, R
Leon-Tavares, J
Lesgourgues, J
Levrier, F
Liguori, M
Lilje, PB
Linden-Vornle, M
Lopez-Caniego, M
Lubin, PM
Macias-Perez, JF
Maggio, G
Maino, D
Mandolesi, N
Mangilli, A
Maris, M
Marshall, DJ
Martin, PG
Martinez-Gonzalez, E
Masi, S
Matarrese, S
McGehee, P
Meinhold, PR
Melchiorri, A
Mendes, L
Mennella, A
Migliaccio, M
Mitra, S
Miville-Deschenes, MA
Moneti, A
Montier, L
Morgante, G
Mortlock, D
Moss, A
Munshi, D
Murphy, JA
Naselsky, P
Nati, F
Natoli, P
Negrello, M
Netterfield, CB
Norgaard-Nielsen, HU
Noviello, F
Novikov, D
Novikov, I
Oxborrow, CA
Paci, F
Pagano, L
Pajot, F
Paladini, R
Paoletti, D
Partridge, B
Pasian, F
Patanchon, G
Pearson, TJ
Perdereau, O
Perotto, L
Perrotta, F
Pettorino, V
Piacentini, F
Piat, M
Pierpaoli, E
Pietrobon, D
Plaszczynski, S
Pointecouteau, E
Polenta, G
Pratt, GW
Prezeau, G
Prunet, S
Puget, JL
Rachen, JP
Reach, WT
Rebolo, R
Reinecke, M
Remazeilles, M
Renault, C
Renzi, A
Ristorcelli, I
Rocha, G
Rosset, C
Rossetti, M
Roudier, G
Rowan-Robinson, M
Rubino-Martin, JA
Rusholme, B
Sandri, M
Sanghera, HS
Santos, D
Savelainen, M
Savini, G
Scott, D
Seiffert, MD
Shellard, EPS
Spencer, LD
Stolyarov, V
Sudiwala, R
Sunyaev, R
Sutton, D
Suur-Uski, AS
Sygnet, JF
Tauber, JA
Terenzi, L
Toffolatti, L
Tomasi, M
Tornikoski, M
Tristram, M
Tucci, M
Tuovinen, J
Turler, M
Umana, G
Valenziano, L
Valiviita, J
Van Tent, B
Vielva, P
Villa, F
Wade, LA
Walter, B
Wandelt, BD
Wehus, IK
Yvon, D
Zacchei, A
Zonca, A
AF Ade, P. A. R.
Aghanim, N.
Argueeso, F.
Arnaud, M.
Ashdown, M.
Aumont, J.
Baccigalupi, C.
Banday, A. J.
Barreiro, R. B.
Bartolo, N.
Battaner, E.
Beichman, C.
Benabed, K.
Benoit, A.
Benoit-Levy, A.
Bernard, J. -P.
Bersanelli, M.
Bielewicz, P.
Bock, J. J.
Boehringer, H.
Bonaldi, A.
Bonavera, L.
Bond, J. R.
Borrill, J.
Bouchet, F. R.
Boulanger, F.
Bucher, M.
Burigana, C.
Butler, R. C.
Calabrese, E.
Cardoso, J. -F.
Carvalho, P.
Catalano, A.
Challinor, A.
Chamballu, A.
Chary, R. -R.
Chiang, H. C.
Christensen, P. R.
Clemens, M.
Clements, D. L.
Colombi, S.
Colombo, L. P. L.
Combet, C.
Couchot, F.
Coulais, A.
Crill, B. P.
Curto, A.
Cuttaia, F.
Danese, L.
Davies, R. D.
Davis, R. J.
de Bernardis, P.
de Rosa, A.
de Zotti, G.
Delabrouille, J.
Desert, F. -X.
Dickinson, C.
Diego, J. M.
Dole, H.
Donzelli, S.
Dore, O.
Douspis, M.
Ducout, A.
Dupac, X.
Efstathiou, G.
Elsner, F.
Ensslin, T. A.
Eriksen, H. K.
Falgarone, E.
Fergusson, J.
Finelli, F.
Forni, O.
Frailis, M.
Fraisse, A. A.
Franceschi, E.
Frejsel, A.
Galeotta, S.
Galli, S.
Ganga, K.
Giard, M.
Giraud-Heraud, Y.
Gjerlow, E.
Gonzalez-Nuevo, J.
Gorski, K. M.
Gratton, S.
Gregorio, A.
Gruppuso, A.
Gudmundsson, J. E.
Hansen, F. K.
Hanson, D.
Harrison, D. L.
Helou, G.
Henrot-Versille, S.
Hernandez-Monteagudo, C.
Herranz, D.
Hildebrandt, S. R.
Hivon, E.
Hobson, M.
Holmes, W. A.
Hornstrup, A.
Hovest, W.
Huffenberger, K. M.
Hurier, G.
Jaffe, A. H.
Jaffe, T. R.
Jones, W. C.
Juvela, M.
Keihanen, E.
Keskitalo, R.
Kisner, T. S.
Kneissl, R.
Knoche, J.
Kunz, M.
Kurki-Suonio, H.
Lagache, G.
Lahteenmaki, A.
Lamarre, J. -M.
Lasenby, A.
Lattanzi, M.
Lawrence, C. R.
Leahy, J. P.
Leonardi, R.
Leon-Tavares, J.
Lesgourgues, J.
Levrier, F.
Liguori, M.
Lilje, P. B.
Linden-Vornle, M.
Lopez-Caniego, M.
Lubin, P. M.
Macias-Perez, J. F.
Maggio, G.
Maino, D.
Mandolesi, N.
Mangilli, A.
Maris, M.
Marshall, D. J.
Martin, P. G.
Martinez-Gonzalez, E.
Masi, S.
Matarrese, S.
McGehee, P.
Meinhold, P. R.
Melchiorri, A.
Mendes, L.
Mennella, A.
Migliaccio, M.
Mitra, S.
Miville-Deschenes, M. -A.
Moneti, A.
Montier, L.
Morgante, G.
Mortlock, D.
Moss, A.
Munshi, D.
Murphy, J. A.
Naselsky, P.
Nati, F.
Natoli, P.
Negrello, M.
Netterfield, C. B.
Norgaard-Nielsen, H. U.
Noviello, F.
Novikov, D.
Novikov, I.
Oxborrow, C. A.
Paci, F.
Pagano, L.
Pajot, F.
Paladini, R.
Paoletti, D.
Partridge, B.
Pasian, F.
Patanchon, G.
Pearson, T. J.
Perdereau, O.
Perotto, L.
Perrotta, F.
Pettorino, V.
Piacentini, F.
Piat, M.
Pierpaoli, E.
Pietrobon, D.
Plaszczynski, S.
Pointecouteau, E.
Polenta, G.
Pratt, G. W.
Prezeau, G.
Prunet, S.
Puget, J. -L.
Rachen, J. P.
Reach, W. T.
Rebolo, R.
Reinecke, M.
Remazeilles, M.
Renault, C.
Renzi, A.
Ristorcelli, I.
Rocha, G.
Rosset, C.
Rossetti, M.
Roudier, G.
Rowan-Robinson, M.
Rubino-Martin, J. A.
Rusholme, B.
Sandri, M.
Sanghera, H. S.
Santos, D.
Savelainen, M.
Savini, G.
Scott, D.
Seiffert, M. D.
Shellard, E. P. S.
Spencer, L. D.
Stolyarov, V.
Sudiwala, R.
Sunyaev, R.
Sutton, D.
Suur-Uski, A. -S.
Sygnet, J. -F.
Tauber, J. A.
Terenzi, L.
Toffolatti, L.
Tomasi, M.
Tornikoski, M.
Tristram, M.
Tucci, M.
Tuovinen, J.
Turler, M.
Umana, G.
Valenziano, L.
Valiviita, J.
Van Tent, B.
Vielva, P.
Villa, F.
Wade, L. A.
Walter, B.
Wandelt, B. D.
Wehus, I. K.
Yvon, D.
Zacchei, A.
Zonca, A.
CA Planck Collaboration
TI Planck 2015 results XXVI. The Second Planck Catalogue of Compact Sources
SO ASTRONOMY & ASTROPHYSICS
LA English
DT Article
DE catalogs; cosmology: observations; radio continuum: general;
submillimeter: general
ID POINT-SOURCE DETECTION; DISCRETE OBJECT DETECTION; HERSCHEL REFERENCE
SURVEY; ACTIVE GALACTIC NUCLEI; ASTRONOMICAL DATA SETS; FAST
BAYESIAN-APPROACH; FLUX-DENSITY SCALE; ALL-SKY SURVEY; EXTRAGALACTIC
SOURCES; NUMBER COUNTS
AB The Second Planck Catalogue of Compact Sources is a list of discrete objects detected in single-frequency maps from the full duration of the Planck mission and supersedes previous versions. It consists of compact sources, both Galactic and extragalactic, detected over the entire sky. Compact sources detected in the lower frequency channels are assigned to the PCCS2, while at higher frequencies they are assigned to one of two subcatalogues, the PCCS2 or PCCS2E, depending on their location on the sky. The first of these (PCCS2) covers most of the sky and allows the user to produce subsamples at higher reliabilities than the target 80% integral reliability of the catalogue. The second ( PCCS2E) contains sources detected in sky regions where the diffuse emission makes it difficult to quantify the reliability of the detections. Both the PCCS2 and PCCS2E include polarization measurements, in the form of polarized flux densities, or upper limits, and orientation angles for all seven polarization-sensitive Planck channels. The improved data-processing of the full-mission maps and their reduced noise levels allow us to increase the number of objects in the catalogue, improving its completeness for the target 80% reliability as compared with the previous versions, the PCCS and the Early Release Compact Source Catalogue (ERCSC).
C1 [Bucher, M.; Cardoso, J. -F.; Delabrouille, J.; Ganga, K.; Giraud-Heraud, Y.; Patanchon, G.; Piat, M.; Remazeilles, M.; Rosset, C.; Roudier, G.] Univ Paris Diderot, APC AstroParticule & Cosmol, CNRS IN2P3, CEA Irfu,Observ Paris,Sorbonne Paris Site, 10 Rue Alice Domon & Leonie Duquet, F-75205 Paris 13, France.
[Leon-Tavares, J.; Tornikoski, M.] Aalto Univ, Metsahovi Radio Observ, POB 13000, Aalto 00076, Finland.
[Lahteenmaki, A.] Dept Radio Sci & Engn, POB 13000, Aalto 00076, Finland.
[Kunz, M.] African Inst Math Sci, 6-8 Melrose Rd, Cape Town, South Africa.
[Natoli, P.; Polenta, G.] Agenzia Spaziale Italiana Sci Data Ctr, Via Politecn Snc, I-00133 Rome, Italy.
[Lagache, G.] Aix Marseille Univ, CNRS, LAM Lab Astrophys Marseille, UMR 7326, F-13388 Marseille, France.
[Ashdown, M.; Curto, A.; Hobson, M.; Lasenby, A.; Stolyarov, V.] Univ Cambridge, Cavendish Lab, Astrophys Grp, JJ Thomson Ave, Cambridge CB3 0HE, England.
[Chiang, H. C.] Univ KwaZulu Natal, Sch Mathe Stat & Comp Sci, Astrophys & Cosmol Res Unit, Westville Campus,Private Bag X54001, ZA-4000 Durban, South Africa.
[Kneissl, R.] ALMA Santiago Cent Off, Atacama Large Millimeter Submillimeter Array, Alonso de Cordova 3107, Santiago 7630355, Chile.
[Leonardi, R.] CGEE, SCS Qd 9,Lote C,Torre C,4 Andar, BR-70308200 Brasilia, DF, Brazil.
[Bond, J. R.; Hanson, D.; Martin, P. G.; Miville-Deschenes, M. -A.] Univ Toronto, CITA, 60 St George St, Toronto, ON M5S 3H8, Canada.
[Banday, A. J.; Bernard, J. -P.; Bielewicz, P.; Forni, O.; Giard, M.; Jaffe, T. R.; Montier, L.; Pointecouteau, E.; Ristorcelli, I.] IRAP, CNRS, 9 Av Colonel Roche,BP 44346, F-31028 Toulouse 4, France.
[Tuovinen, J.] Trinity Coll Dublin, CRANN, Dublin, Ireland.
[Beichman, C.; Bock, J. J.; Crill, B. P.; Dore, O.; Helou, G.; Hildebrandt, S. R.; Pearson, T. J.; Prezeau, G.; Rocha, G.; Seiffert, M. D.] CALTECH, Pasadena, CA 91125 USA.
[Challinor, A.; Fergusson, J.; Shellard, E. P. S.] Univ Cambridge, Ctr Theoret Cosmol, DAMTP, Wilberforce Rd, Cambridge CB3 0WA, England.
[Hernandez-Monteagudo, C.] Ctr Estudios Fis Cosmos Aragon CEFCA, Plaza San Juan 1,Planta 2, Teruel 44001, Spain.
[Borrill, J.; Keskitalo, R.] Lawrence Berkeley Natl Lab, Computat Cosmol Ctr, Berkeley, CA USA.
[Rebolo, R.] CSIC, Madrid, Spain.
[Chamballu, A.; Yvon, D.] CEA Saclay, DSM Irfu SPP, F-91191 Gif Sur Yvette, France.
[Hornstrup, A.; Linden-Vornle, M.; Norgaard-Nielsen, H. U.; Oxborrow, C. A.] Tech Univ Denmark, Natl Space Inst, DTU Space, Elektrovej 327, DK-2800 Lyngby, Denmark.
[Kunz, M.; Tucci, M.] Univ Geneva, Dept Phys Theor, 24 Quai E Ansermet, CH-1211 Geneva 4, Switzerland.
[Rebolo, R.; Rubino-Martin, J. A.] Univ la Laguna, San Cristobal de la Laguna 38206, Tenerife, Spain.
[Gonzalez-Nuevo, J.; Toffolatti, L.] Univ Oviedo, Dept Fis, Avda Calvo Sotelo S-N, Oviedo, Spain.
[Argueeso, F.] Univ Oviedo, Dept Matemat, Avda Calvo Sotelo S-N, Oviedo, Spain.
[Netterfield, C. B.] Univ Toronto, Dept Astron & Astrophys, 50 St George St, Toronto, ON, Canada.
[Rachen, J. P.] Radboud Univ Nijmegen, IMAPP, Dept Astrophys, POB 9010, NL-6500 GL Nijmegen, Netherlands.
[Scott, D.] Univ British Columbia, Dept Phys & Astron, 6224 Agr Rd, Vancouver, BC, Canada.
[Colombo, L. P. L.; Pierpaoli, E.] Univ Southern Calif, Dana & David Dornsife Coll Letter Arts & Sci, Dept Phys & Astron, Los Angeles, CA 90089 USA.
[Benoit-Levy, A.; Elsner, F.] UCL, Dept Phys & Astron, London WC1E 6BT, England.
[Huffenberger, K. M.] Florida State Univ, Dept Phys, Keen Phys Bldg,77 Chieftan Way, Tallahassee, FL 32306 USA.
[Juvela, M.; Keihanen, E.; Kurki-Suonio, H.; Savelainen, M.; Suur-Uski, A. -S.; Valiviita, J.] Univ Helsinki, Dept Phys, Gustaf Hallstromin Katu 2a, Helsinki 00560, Finland.
[Chiang, H. C.; Fraisse, A. A.; Gudmundsson, J. E.; Jones, W. C.; Nati, F.] Princeton Univ, Dept Phys, Princeton, NJ 08544 USA.
[Lubin, P. M.; Meinhold, P. R.; Zonca, A.] Univ Calif Santa Barbara, Dept Phys, Santa Barbara, CA 93106 USA.
[Wandelt, B. D.] Univ Illinois, Dept Phys, 1110 West Green St, Urbana, IL USA.
[Bartolo, N.; Liguori, M.; Matarrese, S.] Univ Padua, Dipartimento Fis & Astron G Galilei, Via Marzolo 8, I-35131 Padua, Italy.
[Burigana, C.; Lattanzi, M.; Mandolesi, N.; Natoli, P.] Univ Ferrara, Dipartimento Fis & Sci Terra, Via Saragat 1, I-44122 Ferrara, Italy.
[de Bernardis, P.; Masi, S.; Melchiorri, A.; Pagano, L.; Piacentini, F.] Univ La Sapienza, Dipartimento Fis, Ple A Moro 2, I-00131 Rome, Italy.
[Bersanelli, M.; Maino, D.; Mennella, A.; Rossetti, M.; Tomasi, M.] Univ Milan, Dipartimento Fis, Via Celoria 16, Milan, Italy.
[Gregorio, A.] Univ Trieste, Dipartimento Fis, Via A Valerio 2, I-34127 Trieste, Italy.
[Renzi, A.] Univ Roma Tor Vergata, Dipartimento Matemat, Via Ric Sci 1, Rome, Italy.
[Christensen, P. R.] Niels Bohr Inst, Discovery Ctr, Blegdamsvej 17, Copenhagen, Denmark.
[Naselsky, P.] Univ Copenhagen, Niels Bohr Inst, Discovery Ctr, Blegdamsvej 17, Copenhagen, Denmark.
[Kneissl, R.] European Southern Observ ESO Vitacura, Alonso de Cordova 3107,Vitacura,Casilla 19001, Santiago, Chile.
[Dupac, X.; Lopez-Caniego, M.; Mendes, L.] European Space Agcy ESAC, Planck Sci Off, Camino Bajo Castillo S-N, Madrid, Spain.
[Tauber, J. A.] European Space Agcy ESTEC, Keplerlaan 1, NL-2201 AZ Noordwijk, Netherlands.
[Leon-Tavares, J.] Univ Turku, Finnish Ctr Astron ESO FINCA, Vaisalantie 20, Piikkio 21500, Finland.
[Matarrese, S.] INFN, Gran Sasso Sci Inst, Viale F Crispi 7, I-67100 Laquila, Italy.
[Pettorino, V.] HGSFP, Philosophenweg 16, D-69120 Heidelberg, Germany.
[Pettorino, V.] Heidelberg Univ, Dept Theoret Phys, Philosophenweg 16, D-69120 Heidelberg, Germany.
[Partridge, B.; Walter, B.] Haverford Coll, Dept Astron, 370 Lancaster Ave, Haverford, PA 19041 USA.
[Kurki-Suonio, H.; Lahteenmaki, A.; Savelainen, M.; Suur-Uski, A. -S.; Valiviita, J.] Univ Helsinki, Helsinki Inst Phys, Gustaf Hallstromin Katu 2, Helsinki 00560, Finland.
[Umana, G.] INAF, Osservatorio Astrofis Catania, Via S Sofia 78, Catania, Italy.
[Clemens, M.; de Zotti, G.; Negrello, M.] INAF, Osservatorio Astron Padova, Vicolo Osservatorio 5, I-35131 Padua, Italy.
[Polenta, G.] INAF, Osservatorio Astron Roma, Via Frascati 33, Monte Porzio Catone, Italy.
[Frailis, M.; Galeotta, S.; Gregorio, A.; Maggio, G.; Maris, M.; Pasian, F.; Zacchei, A.] INAF, Osservatorio Astron Trieste, Via GB Tiepolo 11, I-34127 Trieste, Italy.
[Burigana, C.; Butler, R. C.; Cuttaia, F.; de Rosa, A.; Finelli, F.; Franceschi, E.; Gruppuso, A.; Mandolesi, N.; Morgante, G.; Natoli, P.; Paoletti, D.; Sandri, M.; Terenzi, L.; Toffolatti, L.; Valenziano, L.; Villa, F.] IASF Bologna, INAF, Via Gobetti 101, I-40127 Bologna, Italy.
[Bersanelli, M.; Donzelli, S.; Maino, D.; Mennella, A.; Rossetti, M.; Tomasi, M.] IASF Milano, INAF, Via E Bassini 15, Milan, Italy.
[Burigana, C.; Finelli, F.; Paoletti, D.] INFN, Sez Bologna, Via Irnerio 46, I-40126 Bologna, Italy.
[Melchiorri, A.; Pagano, L.] Univ Roma Sapienza, INFN, Sez Roma 1, Piazzale Aldo Moro 2, I-00185 Rome, Italy.
[Renzi, A.] Univ Roma Tor Vergata, INFN, Sez Roma 2, Via Ric Sci 1, Rome, Italy.
[Gregorio, A.] Ist Nazl Fis Nucl, Nat Inst Nucl Phys, Via Valerio 2, I-34127 Trieste, Italy.
[Desert, F. -X.] Univ Grenoble Alpes, IPAG, CNRS, F-38000 Grenoble, France.
[Turler, M.] Univ Geneva, Dept Astron, ISDC, Ch Ecogia 16, CH-1290 Versoix, Switzerland.
[Mitra, S.] IUCAA, Post Bag 4,Pune Univ Campus, Pune 411007, Maharashtra, India.
[Clements, D. L.; Ducout, A.; Jaffe, A. H.; Mortlock, D.; Rowan-Robinson, M.] Imperial Coll London, Astrophys Grp, Blackett Lab, Prince Consort Rd, London SW7 2AZ, England.
[Chary, R. -R.; McGehee, P.; Paladini, R.; Pearson, T. J.; Rusholme, B.] CALTECH, Infrared Proc & Anal Ctr, Pasadena, CA 91125 USA.
[Benoit, A.] Univ Joseph Fourier Grenoble I, CNRS, Inst Neel, 25 Rue Martyrs, F-91405 Grenoble, France.
[Dole, H.] Inst Univ France, 103 Bd St Michel, F-75005 Paris, France.
[Aghanim, N.; Aumont, J.; Boulanger, F.; Chamballu, A.; Dole, H.; Douspis, M.; Hurier, G.; Kunz, M.; Lagache, G.; Mangilli, A.; Miville-Deschenes, M. -A.; Pajot, F.; Puget, J. -L.; Remazeilles, M.] Univ Paris 11, Univ Paris Saclay, CNRS, Inst Astrophys Spatiale, Bat 121, F-91405 Orsay, France.
[Benabed, K.; Benoit-Levy, A.; Bouchet, F. R.; Cardoso, J. -F.; Colombi, S.; Ducout, A.; Elsner, F.; Hivon, E.; Moneti, A.; Prunet, S.; Sygnet, J. -F.; Wandelt, B. D.] Inst Astrophys Paris, CNRS, UMR7095, 98 Bis Blvd Arago, F-75014 Paris, France.
[Lesgourgues, J.] Rhein Westfal TH Aachen, Inst Theoret Teilchenphys & Kosmol, D-52056 Aachen, Germany.
[Carvalho, P.; Challinor, A.; Efstathiou, G.; Gratton, S.; Harrison, D. L.; Migliaccio, M.; Sanghera, H. S.; Sutton, D.] Univ Cambridge, Inst Astron, Madingley Rd, Cambridge CB3 0HA, England.
[Eriksen, H. K.; Gjerlow, E.; Hansen, F. K.; Lilje, P. B.; Wehus, I. K.] Univ Oslo, Inst Theoret Astrophys, Oslo, Norway.
[Leon-Tavares, J.] Inst Nacl Astrofis Opt & Elect INAOE, Apartado Postal 51 & 216, Puebla 72000, Mexico.
[Rebolo, R.; Rubino-Martin, J. A.] Inst Astrofis Canarias, C Via Lactea S-N, San Cristobal la Laguna, Tenerife, Spain.
[Barreiro, R. B.; Bonavera, L.; Curto, A.; Diego, J. M.; Gonzalez-Nuevo, J.; Herranz, D.; Lopez-Caniego, M.; Martinez-Gonzalez, E.; Toffolatti, L.; Vielva, P.] Univ Cantabria, CSIC, Inst Fis Cantabria, Avda Los Castros S-N, Santander, Spain.
[Bartolo, N.; Liguori, M.; Matarrese, S.] Ist Nazl Fis Nucl, Sez Padova, Via Marzolo 8, I-35131 Padua, Italy.
[Bock, J. J.; Colombo, L. P. L.; Crill, B. P.; Dore, O.; Gorski, K. M.; Hanson, D.; Hildebrandt, S. R.; Holmes, W. A.; Lawrence, C. R.; Mitra, S.; Pietrobon, D.; Prezeau, G.; Rocha, G.; Roudier, G.; Seiffert, M. D.; Wade, L. A.; Wehus, I. K.] CALTECH, Jet Prop Lab, 4800 Oak Grove Dr, Pasadena, CA USA.
[Bonaldi, A.; Davies, R. D.; Davis, R. J.; Dickinson, C.; Leahy, J. P.; Noviello, F.; Remazeilles, M.] Univ Manchester, Sch Phys & Astron, Jodrell Bank Ctr Astrophys, Alan Turing Bldg,Oxford Rd, Manchester M13 9PL, Lancs, England.
[Galli, S.] Univ Chicago, Kavli Inst Cosmol Phys, Chicago, IL 60637 USA.
[Ashdown, M.; Carvalho, P.; Challinor, A.; Curto, A.; Gratton, S.; Harrison, D. L.; Lasenby, A.; Migliaccio, M.; Sanghera, H. S.; Sutton, D.] Kavli Inst Cosmol Cambridge, Madingley Rd, Cambridge CB3 OHA, England.
[Stolyarov, V.] Kazan Fed Univ, 18 Kremlyovskaya St, Kazan 420008, Russia.
[Couchot, F.; Henrot-Versille, S.; Mangilli, A.; Perdereau, O.; Plaszczynski, S.; Tristram, M.] Univ Paris 11, LAL, CNRS IN2P3, F-91405 Orsay, France.
[Catalano, A.; Coulais, A.; Falgarone, E.; Lamarre, J. -M.; Levrier, F.; Roudier, G.] Observ Paris, CNRS, LERMA, 61 Ave Observ, F-75000 Paris, France.
[Arnaud, M.; Chamballu, A.; Marshall, D. J.; Pratt, G. W.] Univ Paris Diderot, CNRS, CEA DSM, Lab AIM,IRFU Serv Astrophys,CEA Saclay, Bat 709, F-91191 Gif Sur Yvette, France.
[Cardoso, J. -F.] CNRS, UMR 5141, Lab Traitement & Commun Informat, 46 Rue Barrault, F-75634 Paris 13, France.
[Cardoso, J. -F.] Telecom ParisTech, 46 Rue Barrault, F-75634 Paris 13, France.
[Catalano, A.; Combet, C.; Macias-Perez, J. F.; Perotto, L.; Renault, C.; Santos, D.] Univ Grenoble Alpes, CNRS IN2P3, Lab Phys Subat & Cosmol, 53 Rue Martyrs, F-38026 Grenoble, France.
[Van Tent, B.] Univ Paris Sud 11, Lab Phys Theor, Batiment 210, F-91405 Orsay, France.
[Van Tent, B.] CNRS, Batiment 210, F-91405 Orsay, France.
[Kisner, T. S.] Lawrence Berkeley Natl Lab, Berkeley, CA USA.
[Novikov, D.; Novikov, I.] Russian Acad Sci, Lebedev Phys Inst, Ctr Astro Space, 84-32 Profsoyuznaya St, Moscow 117997, Russia.
[Ensslin, T. A.; Hernandez-Monteagudo, C.; Hovest, W.; Knoche, J.; Rachen, J. P.; Reinecke, M.; Sunyaev, R.] Max Planck Inst Astrophys, Karl Schwarzschild Str 1, D-85741 Garching, Germany.
[Boehringer, H.] Max Planck Inst Extraterr Phys, Giessenbachstr, D-85748 Garching, Germany.
[Hanson, D.] McGill Univ, McGill Phys, Ernest Rutherford Phys Bldg,3600 Rue Univ, Montreal, PQ H3A 2T8, Canada.
[Murphy, J. A.] Natl Univ Ireland, Dept Expt Phys, Maynooth, Co Kildare, Ireland.
[Bielewicz, P.] Nicolaus Copernicus Astron Ctr, Bartycka 18, PL-00716 Warsaw, Poland.
[Christensen, P. R.; Frejsel, A.; Novikov, I.] Niels Bohr Inst, Blegdamsvej 17, Copenhagen, Denmark.
[Naselsky, P.] Univ Copenhagen, Niels Bohr Inst, Blegdamsvej 17, Copenhagen, Denmark.
[Gudmundsson, J. E.] Nordita Nord Inst Theoret Phys, Roslagstullsbacken 23, S-10691 Stockholm, Sweden.
[Savini, G.] UCL, Opt Sci Lab, Gower St, London, England.
[Baccigalupi, C.; Bielewicz, P.; Danese, L.; de Zotti, G.; Paci, F.; Perrotta, F.] SISSA, Astrophys Sect, Via Bonomea 265, I-34136 Trieste, Italy.
[Terenzi, L.] Univ Studi E Campus, SMARTEST Res Ctr, Via Isimbardi 10, I-22060 Novedrate, CO, Italy.
[Ade, P. A. R.; Munshi, D.; Spencer, L. D.; Sudiwala, R.] Cardiff Univ, Sch Phys & Astron, Queens Bldg, Cardiff CF24 3AA, S Glam, Wales.
[Moss, A.] Univ Nottingham, Sch Phys & Astron, Nottingham NG7 2RD, England.
[Bouchet, F. R.] UPMC, Sorbonne Univ, Inst Astrophys Paris, UMR7095, 98 Bis Blvd Arago, F-75014 Paris, France.
[Sunyaev, R.] Russian Acad Sci, Space Res Inst, IKI, Prof Str 84-32, Moscow 117997, Russia.
[Borrill, J.] Univ Calif Berkeley, Space Sci Lab, Berkeley, CA 94720 USA.
[Stolyarov, V.] Russian Acad Sci, Special Astrophys Observ, Karachai Cherkessian Rep 369167, Russia.
[Calabrese, E.] Univ Oxford, Subdept Astrophys, Keble Rd, Oxford OX1 3RH, England.
[Gudmundsson, J. E.] Stockholm Univ, Dept Phys, Oskar Klein Ctr Cosmoparticle Phys, AlbaNova, S-10691 Stockholm, Sweden.
[Lesgourgues, J.] CERN, PH TH, Div Theory, CH-1211 Geneva 23, Switzerland.
[Benabed, K.; Benoit-Levy, A.; Colombi, S.; Elsner, F.; Hivon, E.; Prunet, S.; Wandelt, B. D.] UPMC Univ Paris 06, UMR7095, 98 Bis Blvd Arago, F-75014 Paris, France.
[Banday, A. J.; Bernard, J. -P.; Forni, O.; Giard, M.; Jaffe, T. R.; Montier, L.; Pointecouteau, E.; Ristorcelli, I.] Univ Toulouse, UPS OMP, IRAP, F-31028 Toulouse 4, France.
[Reach, W. T.] Univ Space Res Assoc, Stratospher Observ Infrared Astron, MS 232-11, Moffett Field, CA 94035 USA.
[Battaner, E.] Univ Granada, Fac Ciencias, Dept Fis Teor & Cosmos, Granada, Spain.
[Battaner, E.] Univ Granada, Inst Carlos I Fis Teor & Computac, Granada, Spain.
[Gorski, K. M.] Univ Warsaw Observ, Aleje Ujazdowskie 4, PL-00478 Warsaw, Poland.
RP Lopez-Caniego, M (reprint author), European Space Agcy ESAC, Planck Sci Off, Camino Bajo Castillo S-N, Madrid, Spain.; Harrison, DL (reprint author), Univ Cambridge, Inst Astron, Madingley Rd, Cambridge CB3 0HA, England.; Lopez-Caniego, M (reprint author), Univ Cantabria, CSIC, Inst Fis Cantabria, Avda Los Castros S-N, Santander, Spain.; Harrison, DL (reprint author), Kavli Inst Cosmol Cambridge, Madingley Rd, Cambridge CB3 OHA, England.
EM dlh@ast.cam.ac.uk; mlopez@sciops.esa.int
RI Lahteenmaki, Anne/L-5987-2013; Barreiro, Rita Belen/N-5442-2014;
bonavera, laura/E-9368-2017; Gonzalez-Nuevo, Joaquin/I-3562-2014;
Herranz, Diego/K-9143-2014; Colombo, Loris/J-2415-2016;
OI Zacchei, Andrea/0000-0003-0396-1192; Toffolatti,
Luigi/0000-0003-2645-7386; Lilje, Per/0000-0003-4324-7794; Paoletti,
Daniela/0000-0003-4761-6147; Nati, Federico/0000-0002-8307-5088; Savini,
Giorgio/0000-0003-4449-9416; Pierpaoli, Elena/0000-0002-7957-8993;
Juvela, Mika/0000-0002-5809-4834; Hurier, Guillaume/0000-0002-1215-0706;
Barreiro, Rita Belen/0000-0002-6139-4272; bonavera,
laura/0000-0001-8039-3876; Kurki-Suonio, Hannu/0000-0002-4618-3063;
Gonzalez-Nuevo, Joaquin/0000-0003-1354-6822; Herranz,
Diego/0000-0003-4540-1417; Colombo, Loris/0000-0003-4572-7732; TERENZI,
LUCA/0000-0001-9915-6379; Stolyarov, Vladislav/0000-0001-8151-828X;
Valiviita, Jussi/0000-0001-6225-3693
FU ESA; CNES (France); CNRS/INSU-IN2P3-INP (France); ASI (Italy); CNR
(Italy); INAF (Italy); NASA (USA); DoE (USA); STFC (UK); UKSA (UK); CSIC
(Spain); MINECO (Spain); JA (Spain); RES (Spain); Tekes (Finland); AoF
(Finland); CSC (Finland); DLR (Germany); MPG (Germany); CSA (Canada);
DTU Space (Denmark); SER/SSO (Switzerland); RCN (Norway); SFI (Ireland);
FCT/MCTES (Portugal); ERC (EU); PRACE (EU); HEFCE
FX The Planck Collaboration acknowledges the support of: ESA; CNES and
CNRS/INSU-IN2P3-INP (France); ASI, CNR, and INAF (Italy); NASA and DoE
(USA); STFC and UKSA (UK); CSIC, MINECO, JA, and, RES (Spain); Tekes,
AoF, and CSC (Finland); DLR and MPG (Germany); CSA (Canada); DTU Space
(Denmark); SER/SSO (Switzerland); RCN (Norway); SFI (Ireland); FCT/MCTES
(Portugal); ERC and PRACE (EU). A description of the Planck
Collaboration and a list of its members, indicating which technical or
scientific activities they have been involved in, can be found at
http://www.cosmos.esa.int/web/planck/planck-collaboration. We are
grateful to the H-ATLAS Executive Committee and primarily to the PIs, S.
Eales and L. Dunne, for permission to use the unpublished H-ATLAS
catalogue for the validation of the present catalogue. This research has
made use of the "Aladin sky atlas" (Bonnarel et al. 2000), developed at
CDS, Strasbourg Observatory, France. Part of this work was performed
using the Darwin Supercomputer of the University of Cambridge High
Performance Computing Service (http://www.hpc.cam.ac.uk/), provided by
Dell Inc. using Strategic Research Infrastructure Funding from the HEFCE
and funding from the STFC. This research has made use of the NASA/IPAC
Extragalactic Database (NED) which is operated by the Jet Propulsion
Laboratory, California Institute of Technology, under contract with the
National Aeronautics and Space Administration.
NR 85
TC 1
Z9 1
U1 1
U2 1
PU EDP SCIENCES S A
PI LES ULIS CEDEX A
PA 17, AVE DU HOGGAR, PA COURTABOEUF, BP 112, F-91944 LES ULIS CEDEX A,
FRANCE
SN 1432-0746
J9 ASTRON ASTROPHYS
JI Astron. Astrophys.
PD OCT
PY 2016
VL 594
AR A26
DI 10.1051/0004-6361/201526914
PG 39
WC Astronomy & Astrophysics
SC Astronomy & Astrophysics
GA DZ4MG
UT WOS:000385832200025
ER
PT J
AU Ade, PAR
Aghanim, N
Alves, MIR
Arnaud, M
Ashdown, M
Aumont, J
Baccigalupi, C
Banday, AJ
Barreiro, RB
Bartlett, JG
Bartolo, N
Battaner, E
Benabed, K
Benoit, A
Benoit-Levy, A
Bernard, JP
Bersanelli, M
Bielewicz, P
Bock, JJ
Bonaldi, A
Bonavera, L
Bond, JR
Borrill, J
Bouchet, FR
Boulanger, F
Bucher, M
Burigana, C
Butler, RC
Calabrese, E
Cardoso, JF
Catalano, A
Challinor, A
Chamballu, A
Chary, RR
Chiang, HC
Christensen, PR
Colombi, S
Colombo, LPL
Combet, C
Couchot, F
Coulais, A
Crill, BP
Curto, A
Cuttaia, F
Danese, L
Davies, RD
Davis, RJ
de Bernardis, P
de Rosa, A
de Zotti, G
Delabrouille, J
Delouis, JM
Desert, FX
Dickinson, C
Diego, JM
Dole, H
Donzelli, S
Dore, O
Douspis, M
Ducout, A
Dupac, X
Efstathiou, G
Elsner, F
Ensslin, TA
Eriksen, HK
Falgarone, E
Fergusson, J
Finelli, F
Forni, O
Frailis, M
Fraisse, AA
Franceschi, E
Frejsel, A
Galeotta, S
Galli, S
Ganga, K
Ghosh, T
Giard, M
Giraud-Heraud, Y
Gjerlow, E
Gonzalez-Nuevo, J
Gorski, KM
Gratton, S
Gregorio, A
Gruppuso, A
Gudmundsson, JE
Hansen, FK
Hanson, D
Harrison, DL
Helou, G
Henrot-Versille, S
Hernandez-Monteagudo, C
Herranz, D
Hildebrandt, SR
Hivon, E
Hobson, M
Holmes, WA
Hornstrup, A
Hovest, W
Huffenberger, KM
Hurier, G
Jaffe, AH
Jaffe, TR
Jones, WC
Juvela, M
Keihanen, E
Keskitalo, R
Kisner, TS
Kneissl, R
Knoche, J
Kunz, M
Kurki-Suonio, H
Lagache, G
Lahteenmaki, A
Lamarre, JM
Lasenby, A
Lattanzi, M
Lawrence, CR
Leahy, JP
Leonardi, R
Lesgourgues, J
Levrier, F
Liguori, M
Lilje, PB
Linden-Vornle, M
Lopez-Caniego, M
Lubin, PM
Macias-Perez, JF
Maggio, G
Maino, D
Mandolesi, N
Mangilli, A
Maris, M
Marshall, DJ
Martin, PG
Martinez-Gonzalez, E
Masi, S
Matarrese, S
McGehee, P
Meinhold, PR
Melchiorri, A
Mendes, L
Mennella, A
Migliaccio, M
Mitra, S
Miville-Deschenes, MA
Moneti, A
Montier, L
Morgante, G
Mortlock, D
Moss, A
Munshi, D
Murphy, JA
Nati, F
Natoli, P
Netterfield, CB
Norgaard-Nielsen, HU
Noviello, F
Novikov, D
Novikov, I
Orlando, E
Oxborrow, CA
Paci, F
Pagano, L
Pajot, F
Paladini, R
Paoletti, D
Partridge, B
Pasian, F
Patanchon, G
Pearson, TJ
Peel, M
Perdereau, O
Perotto, L
Perrotta, F
Pettorino, V
Piacentini, F
Piat, M
Pierpaoli, E
Pietrobon, D
Plaszczynski, S
Pointecouteau, E
Polenta, G
Pratt, GW
Prezeau, G
Prunet, S
Puget, JL
Rachen, JP
Reach, WT
Rebolo, R
Reinecke, M
Remazeilles, M
Renault, C
Renzi, A
Ristorcelli, I
Rocha, G
Rosset, C
Rossetti, M
Roudier, G
Rubino-Martin, JA
Rusholme, B
Sandri, M
Santos, D
Savelainen, M
Savini, G
Scott, D
Seiffert, MD
Shellard, EPS
Spencer, LD
Stolyarov, V
Stompor, R
Strong, AW
Sudiwala, R
Sunyaev, R
Sutton, D
Suur-Uski, AS
Sygnet, JF
Tauber, JA
Terenzi, L
Toffolatti, L
Tomasi, M
Tristram, M
Tucci, M
Tuovinen, J
Umana, G
Valenziano, L
Valiviita, J
Van Tent, F
Vidal, M
Vielva, P
Villa, F
Wade, LA
Wandelt, BD
Watson, R
Wehus, IK
Wilkinson, A
Yvon, D
Zacchei, A
Zonca, A
AF Ade, P. A. R.
Aghanim, N.
Alves, M. I. R.
Arnaud, M.
Ashdown, M.
Aumont, J.
Baccigalupi, C.
Banday, A. J.
Barreiro, R. B.
Bartlett, J. G.
Bartolo, N.
Battaner, E.
Benabed, K.
Benoit, A.
Benoit-Levy, A.
Bernard, J. -P.
Bersanelli, M.
Bielewicz, P.
Bock, J. J.
Bonaldi, A.
Bonavera, L.
Bond, J. R.
Borrill, J.
Bouchet, F. R.
Boulanger, F.
Bucher, M.
Burigana, C.
Butler, R. C.
Calabrese, E.
Cardoso, J. -F.
Catalano, A.
Challinor, A.
Chamballu, A.
Chary, R. -R.
Chiang, H. C.
Christensen, P. R.
Colombi, S.
Colombo, L. P. L.
Combet, C.
Couchot, F.
Coulais, A.
Crill, B. P.
Curto, A.
Cuttaia, F.
Danese, L.
Davies, R. D.
Davis, R. J.
de Bernardis, P.
de Rosa, A.
de Zotti, G.
Delabrouille, J.
Delouis, J. -M.
Desert, F. -X.
Dickinson, C.
Diego, J. M.
Dole, H.
Donzelli, S.
Dore, O.
Douspis, M.
Ducout, A.
Dupac, X.
Efstathiou, G.
Elsner, F.
Ensslin, T. A.
Eriksen, H. K.
Falgarone, E.
Fergusson, J.
Finelli, F.
Forni, O.
Frailis, M.
Fraisse, A. A.
Franceschi, E.
Frejsel, A.
Galeotta, S.
Galli, S.
Ganga, K.
Ghosh, T.
Giard, M.
Giraud-Heraud, Y.
Gjerlow, E.
Gonzalez-Nuevo, J.
Gorski, K. M.
Gratton, S.
Gregorio, A.
Gruppuso, A.
Gudmundsson, J. E.
Hansen, F. K.
Hanson, D.
Harrison, D. L.
Helou, G.
Henrot-Versille, S.
Hernandez-Monteagudo, C.
Herranz, D.
Hildebrandt, S. R.
Hivon, E.
Hobson, M.
Holmes, W. A.
Hornstrup, A.
Hovest, W.
Huffenberger, K. M.
Hurier, G.
Jaffe, A. H.
Jaffe, T. R.
Jones, W. C.
Juvela, M.
Keihanen, E.
Keskitalo, R.
Kisner, T. S.
Kneissl, R.
Knoche, J.
Kunz, M.
Kurki-Suonio, H.
Lagache, G.
Lahteenmaki, A.
Lamarre, J. -M.
Lasenby, A.
Lattanzi, M.
Lawrence, C. R.
Leahy, J. P.
Leonardi, R.
Lesgourgues, J.
Levrier, F.
Liguori, M.
Lilje, P. B.
Linden-Vornle, M.
Lopez-Caniego, M.
Lubin, P. M.
Macias-Perez, J. F.
Maggio, G.
Maino, D.
Mandolesi, N.
Mangilli, A.
Maris, M.
Marshall, D. J.
Martin, P. G.
Martinez-Gonzalez, E.
Masi, S.
Matarrese, S.
McGehee, P.
Meinhold, P. R.
Melchiorri, A.
Mendes, L.
Mennella, A.
Migliaccio, M.
Mitra, S.
Miville-Deschenes, M. -A.
Moneti, A.
Montier, L.
Morgante, G.
Mortlock, D.
Moss, A.
Munshi, D.
Murphy, J. A.
Nati, F.
Natoli, P.
Netterfield, C. B.
Norgaard-Nielsen, H. U.
Noviello, F.
Novikov, D.
Novikov, I.
Orlando, E.
Oxborrow, C. A.
Paci, F.
Pagano, L.
Pajot, F.
Paladini, R.
Paoletti, D.
Partridge, B.
Pasian, F.
Patanchon, G.
Pearson, T. J.
Peel, M.
Perdereau, O.
Perotto, L.
Perrotta, F.
Pettorino, V.
Piacentini, F.
Piat, M.
Pierpaoli, E.
Pietrobon, D.
Plaszczynski, S.
Pointecouteau, E.
Polenta, G.
Pratt, G. W.
Prezeau, G.
Prunet, S.
Puget, J. -L.
Rachen, J. P.
Reach, W. T.
Rebolo, R.
Reinecke, M.
Remazeilles, M.
Renault, C.
Renzi, A.
Ristorcelli, I.
Rocha, G.
Rosset, C.
Rossetti, M.
Roudier, G.
Rubino-Martin, J. A.
Rusholme, B.
Sandri, M.
Santos, D.
Savelainen, M.
Savini, G.
Scott, D.
Seiffert, M. D.
Shellard, E. P. S.
Spencer, L. D.
Stolyarov, V.
Stompor, R.
Strong, A. W.
Sudiwala, R.
Sunyaev, R.
Sutton, D.
Suur-Uski, A. -S.
Sygnet, J. -F.
Tauber, J. A.
Terenzi, L.
Toffolatti, L.
Tomasi, M.
Tristram, M.
Tucci, M.
Tuovinen, J.
Umana, G.
Valenziano, L.
Valiviita, J.
Van Tent, F.
Vidal, M.
Vielva, P.
Villa, F.
Wade, L. A.
Wandelt, B. D.
Watson, R.
Wehus, I. K.
Wilkinson, A.
Yvon, D.
Zacchei, A.
Zonca, A.
CA Planck Collaboration
TI Planck 2015 results XXV. Diffuse low-frequency Galactic foregrounds
SO ASTRONOMY & ASTROPHYSICS
LA English
DT Article
DE diffuse radiation; ISM: general; radiation mechanisms: general; radio
continuum: ISM; polarization; local insterstellar matter
ID MICROWAVE-ANISOTROPY-PROBE; NORTH-POLAR SPUR; LARGE-MAGELLANIC-CLOUD;
PERSEUS MOLECULAR-COMPLEX; BAYESIAN COMPONENT SEPARATION;
CENTIMETER-WAVE CONTINUUM; COSMIC-RAY PROPAGATION; LAMBDA-ORIONIS RING;
ALL-SKY SURVEY; RADIO-CONTINUUM
AB We discuss the Galactic foreground emission between 20 and 100 GHz based on observations by Planck and WMAP. The total intensity in this part of the spectrum is dominated by free-free and spinning dust emission, whereas the polarized intensity is dominated by synchrotron emission. The Commander component-separation tool has been used to separate the various astrophysical processes in total intensity. Comparison with radio recombination line templates verifies the recovery of the free-free emission along the Galactic plane. Comparison of the high-latitude H alpha emission with our free-free map shows residuals that correlate with dust optical depth, consistent with a fraction (approximate to 30%) of H alpha having been scattered by high-latitude dust. We highlight a number of diffuse spinning dust morphological features at high latitude. There is substantial spatial variation in the spinning dust spectrum, with the emission peak (in I-v) ranging from below 20 GHz to more than 50 GHz. There is a strong tendency for the spinning dust component near many prominent H Pi regions to have a higher peak frequency, suggesting that this increase in peak frequency is associated with dust in the photo-dissociation regions around the nebulae. The emissivity of spinning dust in these diffuse regions is of the same order as previous detections in the literature. Over the entire sky, the Commander solution finds more anomalous microwave emission (AME) than the WMAP component maps, at the expense of synchrotron and free-free emission. This can be explained by the difficulty in separating multiple broadband components with a limited number of frequency maps. Future surveys, particularly at 5-20 GHz, will greatly improve the separation by constraining the synchrotron spectrum. We combine Planck and WMAP data to make the highest signal-to-noise ratio maps yet of the intensity of the all-sky polarized synchrotron emission at frequencies above a few GHz. Most of the high-latitude polarized emission is associated with distinct large-scale loops and spurs, and we re-discuss their structure. We argue that nearly all the emission at 40 degrees > l > -90 degrees is part of the Loop I structure, and show that the emission extends much further in to the southern Galactic hemisphere than previously recognised, giving Loop I an ovoid rather than circular outline. However, it does not continue as far as the "Fermi bubble/microwave haze", making it less probable that these are part of the same structure. We identify a number of new faint features in the polarized sky, including a dearth of polarized synchrotron emission directly correlated with a narrow, roughly 20 degrees long filament seen in H alpha at high Galactic latitude. Finally, we look for evidence of polarized AME, however many AME regions are significantly contaminated by polarized synchrotron emission, and we find a 2 sigma upper limit of 1.6% in the Perseus region.
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[Gudmundsson, J. E.] Stockholm Univ, AlbaNova, Oskar Klein Ctr Cosmoparticle Phys, Dept Phys, S-10691 Stockholm, Sweden.
[Lesgourgues, J.] CERN, PH TH, Div Theory, CH-1211 Geneva 23, Switzerland.
[Benabed, K.; Benoit-Levy, A.; Colombi, S.; Delouis, J. -M.; Elsner, F.; Hivon, E.; Prunet, S.; Wandelt, B. D.] Univ Paris 06, UMR7095, 98 Bis Blvd Arago, F-75014 Paris, France.
[Alves, M. I. R.; Banday, A. J.; Bernard, J. -P.; Forni, O.; Giard, M.; Jaffe, T. R.; Montier, L.; Pointecouteau, E.; Ristorcelli, I.] Univ Toulouse, UPS OMP, TRAP, F-31028 Toulouse, France.
[Reach, W. T.] Univ Space Res Assoc, Stratospher Observ Infrared Astron, MS 232-11, Moffett Field, CA 94035 USA.
[Battaner, E.] Univ Granada, Fac Ciencias, Dept Fis Teor & Cosmos, E-18071 Granada, Spain.
[Battaner, E.] Univ Granada, Inst Carlos Fis Teor & Computac 1, E-18071 Granada, Spain.
[Orlando, E.] Stanford Univ, Kavli Inst Particle Astrophys & Cosmol, Dept Phys, WW Hansen Expt Phys Lab, Stanford, CA 94305 USA.
[Orlando, E.] Stanford Univ, SLAC Natl Accelerator Lab, Stanford, CA 94305 USA.
[Gorski, K. M.] Univ Warsaw Observ, Aleje Ujazdowskie 4, PL-00478 Warsaw, Poland.
RP Dickinson, C; Leahy, JP (reprint author), Univ Manchester, Jodrell Bank Ctr Astrophys, Sch Phys & Astron, Alan Turing Bldg,Oxford Rd, Manchester M13 9PL, Lancs, England.
EM Clive.dickinson@manchester.ac.uk; j.p.leahy@manchester.ac.uk
RI Lahteenmaki, Anne/L-5987-2013; Barreiro, Rita Belen/N-5442-2014;
bonavera, laura/E-9368-2017; Gonzalez-Nuevo, Joaquin/I-3562-2014;
Herranz, Diego/K-9143-2014; Colombo, Loris/J-2415-2016;
OI Barreiro, Rita Belen/0000-0002-6139-4272; bonavera,
laura/0000-0001-8039-3876; Gonzalez-Nuevo, Joaquin/0000-0003-1354-6822;
Herranz, Diego/0000-0003-4540-1417; Colombo, Loris/0000-0003-4572-7732;
TERENZI, LUCA/0000-0001-9915-6379; Stolyarov,
Vladislav/0000-0001-8151-828X; Valiviita, Jussi/0000-0001-6225-3693;
Hurier, Guillaume/0000-0002-1215-0706; Kurki-Suonio,
Hannu/0000-0002-4618-3063; Zacchei, Andrea/0000-0003-0396-1192; Hivon,
Eric/0000-0003-1880-2733; Toffolatti, Luigi/0000-0003-2645-7386; Lilje,
Per/0000-0003-4324-7794; Paoletti, Daniela/0000-0003-4761-6147; Nati,
Federico/0000-0002-8307-5088; Savini, Giorgio/0000-0003-4449-9416;
Pierpaoli, Elena/0000-0002-7957-8993; Juvela, Mika/0000-0002-5809-4834
FU ESA; CNES (France); CNRS/INSU-IN2P3-INP (France); ASI (Italy); CNR
(Italy); INAF (Italy); NASA (USA); DoE (USA); STFC (UK); UKSA (UK); CSIC
(Spain); MINECO (Spain); JA (Spain); RES (Spain); Tekes (Finland); AoF
(Finland); CSC (Finland); DLR (Germany); MPG (Germany); CSA (Canada);
DTU Space (Denmark); SER/SSO (Switzerland); RCN (Norway); SFI (Ireland);
FCT/MCTES (Portugal); ERC (EU); PRACE (EU); ERC [307209]; STFC
Consolidated Grant [ST/L000768/1]
FX This paper is dedicated to the memory of the late Professor Rodney Deane
Davies CBE FRS and Professor Richard John Davis OBE, both of whom
contributed greatly to the Planck project. The Planck Collaboration
acknowledges the support of: ESA; CNES and CNRS/INSU-IN2P3-INP (France);
ASI, CNR, and INAF (Italy); NASA and DoE (USA); STFC and UKSA (UK);
CSIC, MINECO, JA, and RES (Spain); Tekes, AoF, and CSC (Finland); DLR
and MPG (Germany); CSA (Canada); DTU Space (Denmark); SER/SSO
(Switzerland); RCN (Norway); SFI (Ireland); FCT/MCTES (Portugal); ERC
and PRACE (EU). A description of the Planck Collaboration and a list of
its members, indicating which technical or scientific activities they
have been involved in, can be found at
http://www.cosmos.esa.int/web/planck/planck-collaboration. This research
was supported by an ERC Starting (Consolidator) Grant (no. 307209) and
STFC Consolidated Grant (no. ST/L000768/1). We have made extensive use
of the HEALPix package and the IDL astronomy library. This research has
made use of the SIMBAD database, operated at CDS, Strasbourg, France.
NR 227
TC 1
Z9 1
U1 0
U2 0
PU EDP SCIENCES S A
PI LES ULIS CEDEX A
PA 17, AVE DU HOGGAR, PA COURTABOEUF, BP 112, F-91944 LES ULIS CEDEX A,
FRANCE
SN 1432-0746
J9 ASTRON ASTROPHYS
JI Astron. Astrophys.
PD OCT
PY 2016
VL 594
AR A25
DI 10.1051/0004-6361/201526803
PG 45
WC Astronomy & Astrophysics
SC Astronomy & Astrophysics
GA DZ4MG
UT WOS:000385832200024
ER
PT J
AU Ade, PAR
Aghanim, N
Ashdown, M
Aumont, J
Baccigalupi, C
Banday, AJ
Barreiro, RB
Bartolo, N
Battaglia, P
Battaner, E
Benabed, K
Benoit, A
Benoit-Levy, A
Bernard, JP
Bersanelli, M
Bielewicz, P
Bock, JJ
Bonaldi, A
Bonavera, L
Bond, JR
Borrill, J
Bouchet, FR
Bucher, M
Burigana, C
Butler, RC
Calabrese, E
Cardoso, JF
Catalano, A
Chamballu, A
Christensen, PR
Colombi, S
Colombo, LPL
Crill, BP
Curto, A
Cuttaia, F
Danese, L
Davies, RD
Davis, RJ
de Bernardis, P
de Rosa, A
de Zotti, G
Delabrouille, J
Dickinson, C
Diego, JM
Dole, H
Donzelli, S
Dore, O
Douspis, M
Ducout, A
Dupac, X
Efstathiou, G
Elsner, F
Ensslin, TA
Eriksen, HK
Fergusson, J
Finelli, F
Forni, O
Frailis, M
Franceschi, E
Frejsel, A
Galeotta, S
Galli, S
Ganga, K
Giard, M
Giraud-Heraud, Y
Gjerlow, E
Gonzalez-Nuevo, J
Gorski, KM
Gratton, S
Gregorio, A
Gruppuso, A
Hansen, FK
Hanson, D
Harrison, DL
Henrot-Versille, S
Herranz, D
Hildebrandt, SR
Hivon, E
Hobson, M
Holmes, WA
Hornstrup, A
Hovest, W
Huffenberger, KM
Hurier, G
Jaffe, AH
Jaffe, TR
Juvela, M
Keihanen, E
Keskitalo, R
Kisner, TS
Knoche, J
Krachmalnicoff, N
Kunz, M
Kurki-Suonio, H
Lagache, G
Lahteenmaki, A
Lamarre, JM
Lasenby, A
Lattanzi, M
Lawrence, CR
Leahy, JP
Leonardi, R
Lesgourgues, J
Levrier, F
Liguori, M
Lilje, PB
Linden-Vornle, M
Lopez-Caniego, M
Lubin, PM
Macias-Perez, JF
Maggio, G
Maino, D
Mandolesi, N
Mangilli, A
Maris, M
Martin, PG
Martinez-Gonzalez, E
Masi, S
Matarrese, S
McGehee, P
Meinhold, PR
Melchiorri, A
Mendes, L
Mennella, A
Migliaccio, M
Mitra, S
Montier, L
Morgante, G
Mortlock, D
Moss, A
Munshi, D
Murphy, JA
Naselsky, P
Nati, F
Natoli, P
Netterfield, CB
Norgaard-Nielsen, HU
Novikov, D
Novikov, I
Paci, F
Pagano, L
Pajot, F
Paoletti, D
Partridge, B
Pasian, F
Patanchon, G
Pearson, TJ
Peel, M
Perdereau, O
Perotto, L
Perrotta, F
Pettorino, V
Piacentini, F
Pierpaoli, E
Pietrobon, D
Pointecouteau, E
Polenta, G
Pratt, GW
Prezeau, G
Prunet, S
Puget, JL
Rachen, JP
Rebolo, R
Reinecke, M
Remazeilles, M
Renzi, A
Rocha, G
Romelli, E
Rosset, C
Rossetti, M
Roudier, G
Rubino-Martin, JA
Rusholme, B
Sandri, M
Santos, D
Savelainen, M
Scott, D
Seiffert, MD
Shellard, EPS
Spencer, LD
Stolyarov, V
Sutton, D
Suur-Uski, AS
Sygnet, JF
Tauber, JA
Tavagnacco, D
Terenzi, L
Toffolatti, L
Tomasi, M
Tristram, M
Tucci, M
Tuovinen, J
Turler, M
Umana, G
Valenziano, L
Valiviita, J
Van Tent, B
Vassallo, T
Vielva, P
Villa, F
Wade, LA
Wandelt, BD
Watson, R
Wehus, IK
Wilkinson, A
Yvon, D
Zacchei, A
Zonca, A
AF Ade, P. A. R.
Aghanim, N.
Ashdown, M.
Aumont, J.
Baccigalupi, C.
Banday, A. J.
Barreiro, R. B.
Bartolo, N.
Battaglia, P.
Battaner, E.
Benabed, K.
Benoit, A.
Benoit-Levy, A.
Bernard, J. -P.
Bersanelli, M.
Bielewicz, P.
Bock, J. J.
Bonaldi, A.
Bonavera, L.
Bond, J. R.
Borrill, J.
Bouchet, F. R.
Bucher, M.
Burigana, C.
Butler, R. C.
Calabrese, E.
Cardoso, J. -F.
Catalano, A.
Chamballu, A.
Christensen, P. R.
Colombi, S.
Colombo, L. P. L.
Crill, B. P.
Curto, A.
Cuttaia, F.
Danese, L.
Davies, R. D.
Davis, R. J.
de Bernardis, P.
de Rosa, A.
de Zotti, G.
Delabrouille, J.
Dickinson, C.
Diego, J. M.
Dole, H.
Donzelli, S.
Dore, O.
Douspis, M.
Ducout, A.
Dupac, X.
Efstathiou, G.
Elsner, F.
Ensslin, T. A.
Eriksen, H. K.
Fergusson, J.
Finelli, F.
Forni, O.
Frailis, M.
Franceschi, E.
Frejsel, A.
Galeotta, S.
Galli, S.
Ganga, K.
Giard, M.
Giraud-Heraud, Y.
Gjerlow, E.
Gonzalez-Nuevo, J.
Gorski, K. M.
Gratton, S.
Gregorio, A.
Gruppuso, A.
Hansen, F. K.
Hanson, D.
Harrison, D. L.
Henrot-Versille, S.
Herranz, D.
Hildebrandt, S. R.
Hivon, E.
Hobson, M.
Holmes, W. A.
Hornstrup, A.
Hovest, W.
Huffenberger, K. M.
Hurier, G.
Jaffe, A. H.
Jaffe, T. R.
Juvela, M.
Keihanen, E.
Keskitalo, R.
Kisner, T. S.
Knoche, J.
Krachmalnicoff, N.
Kunz, M.
Kurki-Suonio, H.
Lagache, G.
Lahteenmaki, A.
Lamarre, J. -M.
Lasenby, A.
Lattanzi, M.
Lawrence, C. R.
Leahy, J. P.
Leonardi, R.
Lesgourgues, J.
Levrier, F.
Liguori, M.
Lilje, P. B.
Linden-Vornle, M.
Lopez-Caniego, M.
Lubin, P. M.
Macias-Perez, J. F.
Maggio, G.
Maino, D.
Mandolesi, N.
Mangilli, A.
Maris, M.
Martin, P. G.
Martinez-Gonzalez, E.
Masi, S.
Matarrese, S.
McGehee, P.
Meinhold, P. R.
Melchiorri, A.
Mendes, L.
Mennella, A.
Migliaccio, M.
Mitra, S.
Montier, L.
Morgante, G.
Mortlock, D.
Moss, A.
Munshi, D.
Murphy, J. A.
Naselsky, P.
Nati, F.
Natoli, P.
Netterfield, C. B.
Norgaard-Nielsen, H. U.
Novikov, D.
Novikov, I.
Paci, F.
Pagano, L.
Pajot, F.
Paoletti, D.
Partridge, B.
Pasian, F.
Patanchon, G.
Pearson, T. J.
Peel, M.
Perdereau, O.
Perotto, L.
Perrotta, F.
Pettorino, V.
Piacentini, F.
Pierpaoli, E.
Pietrobon, D.
Pointecouteau, E.
Polenta, G.
Pratt, G. W.
Prezeau, G.
Prunet, S.
Puget, J. -L.
Rachen, J. P.
Rebolo, R.
Reinecke, M.
Remazeilles, M.
Renzi, A.
Rocha, G.
Romelli, E.
Rosset, C.
Rossetti, M.
Roudier, G.
Rubino-Martin, J. A.
Rusholme, B.
Sandri, M.
Santos, D.
Savelainen, M.
Scott, D.
Seiffert, M. D.
Shellard, E. P. S.
Spencer, L. D.
Stolyarov, V.
Sutton, D.
Suur-Uski, A. -S.
Sygnet, J. -F.
Tauber, J. A.
Tavagnacco, D.
Terenzi, L.
Toffolatti, L.
Tomasi, M.
Tristram, M.
Tucci, M.
Tuovinen, J.
Turler, M.
Umana, G.
Valenziano, L.
Valiviita, J.
Van Tent, B.
Vassallo, T.
Vielva, P.
Villa, F.
Wade, L. A.
Wandelt, B. D.
Watson, R.
Wehus, I. K.
Wilkinson, A.
Yvon, D.
Zacchei, A.
Zonca, A.
CA Planck Collaboration
TI Planck 2015 results V. LFI calibration
SO ASTRONOMY & ASTROPHYSICS
LA English
DT Article
DE cosmic background radiation; instrumentation: polarimeters; methods:
data analysis
ID PROBE WMAP OBSERVATIONS; SYSTEMATIC-ERROR LIMITS; PRE-LAUNCH STATUS;
BEAM PROFILES; MICROWAVE; MAPS
AB We present a description of the pipeline used to calibrate the Planck Low Frequency Instrument (LFI) timelines into thermodynamic temperatures for the Planck 2015 data release, covering four years of uninterrupted operations. As in the 2013 data release, our calibrator is provided by the spin-synchronous modulation of the cosmic microwave background dipole, but we now use the orbital component, rather than adopting the Wilkinson Microwave Anisotropy Probe (WMAP) solar dipole. This allows our 2015 LFI analysis to provide an independent Solar dipole estimate, which is in excellent agreement with that of HFI and within 1 sigma (0.3% in amplitude) of the WMAP value. This 0.3% shift in the peak-to-peak dipole temperature from WMAP and a general overhaul of the iterative calibration code increases the overall level of the LFI maps by 0.45% (30 GHz), 0.64% (44 GHz), and 0.82% (70 GHz) in temperature with respect to the 2013 Planck data release, thus reducing the discrepancy with the power spectrum measured by WMAP. We estimate that the LFI calibration uncertainty is now at the level of 0.20% for the 70 GHz map, 0.26% for the 44 GHz map, and 0.35% for the 30 GHz map. We provide a detailed description of the impact of all the changes implemented in the calibration since the previous data release.
C1 [Bucher, M.; Cardoso, J. -F.; Delabrouille, J.; Ganga, K.; Giraud-Heraud, Y.; Patanchon, G.; Remazeilles, M.; Rosset, C.; Roudier, G.] Univ Paris Diderot, CNRS IN2P3, CEA Irfu, APC AstroParticule & Cosmol,Observ Paris,Sorbonne, 10 rue Alice Domon & Leonie Duquet, F-75205 Paris 13, France.
[Lahteenmaki, A.] Aalto Univ, Metsahovi Radio Observ, POB 13000, Aalto 00076, Finland.
[Lahteenmaki, A.] Dept Radio Sci & Engn, POB 13000, Aalto 00076, Finland.
[Kunz, M.] African Inst Math Sci, 6-8 Melrose Rd, Cape Town, South Africa.
[Natoli, P.; Polenta, G.] Agenzia Spaziale Italiana Sci Data Ctr, Via Politecn Snc, I-00133 Rome, Italy.
[Lagache, G.] Aix Marseille Univ, CNRS, LAM, UMR 7326, F-13388 Marseille, France.
[Ashdown, M.; Curto, A.; Hobson, M.; Lasenby, A.; Stolyarov, V.] Univ Cambridge, Cavendish Lab, Astrophys Grp, JJ Thomson Ave, Cambridge CB3 0HE, England.
[Leonardi, R.] CGEE, SCS Qd 9, Lote C,Torre C,4 Andar,Ed Parque Cidade Corp, BR-70308200 Brasilia, DF, Brazil.
[Bond, J. R.; Hanson, D.; Martin, P. G.] Univ Toronto, CITA, 60 St George St, Toronto, ON M5S 3H8, Canada.
[Banday, A. J.; Bernard, J. -P.; Bielewicz, P.; Forni, O.; Giard, M.; Jaffe, T. R.; Montier, L.; Pointecouteau, E.] CNRS, IRAP, 9 Av Colonel Roche,BP 44346, F-31028 Toulouse 4, France.
[Tuovinen, J.] Trinity Coll Dublin, CRANN, Dublin, Ireland.
[Bock, J. J.; Crill, B. P.; Dore, O.; Hildebrandt, S. R.; Pearson, T. J.; Prezeau, G.; Rocha, G.; Seiffert, M. D.] CALTECH, Pasadena, CA 91125 USA.
[Fergusson, J.; Shellard, E. P. S.] Univ Cambridge, Ctr Theoret Cosmol, DAMTP, Wilberforce Rd, Cambridge CB3 0WA, England.
[Borrill, J.; Keskitalo, R.] Lawrence Berkeley Natl Lab, Computat Cosmol Ctr, Berkeley, CA USA.
[Rebolo, R.] CSIC, Madrid, Spain.
[Chamballu, A.; Yvon, D.] CEA Saclay, DSM Irfu SPP, F-91191 Gif Sur Yvette, France.
[Hornstrup, A.; Linden-Vornle, M.; Norgaard-Nielsen, H. U.] Tech Univ Denmark, Natl Space Inst, DTU Space, Elektrovej 327, DK-2800 Lyngby, Denmark.
[Kunz, M.; Tucci, M.] Univ Geneva, Dept Phys Theor, 24 Quai E Ansermet, CH-1211 Geneva 4, Switzerland.
[Rebolo, R.; Rubino-Martin, J. A.] Univ La Laguna, Dept Astrofis, San Cristobal la Laguna 38206, Tenerife, Spain.
[Gonzalez-Nuevo, J.; Toffolatti, L.] Univ Oviedo, Dept Fis, Avda Calvo Sotelo S-N, Oviedo, Spain.
[Netterfield, C. B.] Univ Toronto, Dept Astron & Astrophys, 50 St George St, Toronto, ON, Canada.
[Rachen, J. P.] Radboud Univ Nijmegen, IMAPP, Dept Astrophys, POB 9010, NL-6500 GL Nijmegen, Netherlands.
[Scott, D.] Univ British Columbia, Dept Phys & Astron, 6224 Agr Rd, Vancouver, BC, Canada.
[Colombo, L. P. L.; Pierpaoli, E.] Univ Southern Calif, Dana & David Dornsife Coll Letter Arts & Sci, Dept Phys & Astron, Los Angeles, CA 90089 USA.
[Benoit-Levy, A.; Elsner, F.] UCL, Dept Phys & Astron, London WC1E 6BT, England.
[Huffenberger, K. M.] Florida State Univ, Dept Phys, Keen Phys Bldg,77 Chieftan Way, Tallahassee, FL 32306 USA.
[Juvela, M.; Keihanen, E.; Kurki-Suonio, H.; Savelainen, M.; Suur-Uski, A. -S.; Valiviita, J.] Univ Helsinki, Dept Phys, Gustaf Hallstromin Katu 2a, Helsinki, Finland.
[Nati, F.] Princeton Univ, Dept Phys, Princeton, NJ 08544 USA.
[Lubin, P. M.; Meinhold, P. R.; Zonca, A.] Univ Calif Santa Barbara, Dept Phys, Santa Barbara, CA 93106 USA.
[Wandelt, B. D.] Univ Illinois, Dept Phys, 1110 West Green St, Urbana, IL USA.
[Bartolo, N.; Liguori, M.; Matarrese, S.] Univ Padua, Dipartimento Fis & Astron G Galilei, Via Marzolo 8, I-35131 Padua, Italy.
[Burigana, C.; Lattanzi, M.; Mandolesi, N.; Natoli, P.] Univ Ferrara, Dipartimento Fis & Sci Terra, Via Saragat 1, I-44122 Ferrara, Italy.
[Battaglia, P.; de Bernardis, P.; Masi, S.; Melchiorri, A.; Pagano, L.; Piacentini, F.] Univ Roma La Sapienza, Dipartimento Fis, Ple A Moro 2, I-00185 Rome, Italy.
[Bersanelli, M.; Krachmalnicoff, N.; Kunz, M.; Maino, D.; Mennella, A.; Rossetti, M.; Tomasi, M.] Univ Milan, Dipartimento Fis, Via Celoria 16, I-20133 Milan, Italy.
[Battaglia, P.; Gregorio, A.; Romelli, E.; Tavagnacco, D.] Univ Trieste, Dipartimento Fis, Via A Valerio 2, I-34127 Trieste, Italy.
[Renzi, A.] Univ Roma Tor Vergata, Dipartimento Matemat, Via Ric Sci 1, I-00185 Rome, Italy.
[Christensen, P. R.] Niels Bohr Inst, Discovery Ctr, Blegdamsvej 17, DK-1165 Copenhagen, Denmark.
[Naselsky, P.] Univ Copenhagen, Niels Bohr Inst, Discovery Ctr, Blegdamsvej 17, DK-1165 Copenhagen, Denmark.
[Dupac, X.; Lopez-Caniego, M.; Mendes, L.] European Space Agcy, ESAC, Planck Sci Off, Camino Bajo Castillo S-N, Madrid 68692, Spain.
[Tauber, J. A.] European Space Agcy, Estec, Keplerlaan 1, NL-2201 AZ Noordwijk, Netherlands.
[Matarrese, S.] Ist Nazl Fis Nucl, Gran Sasso Sci Inst, Viale F Crispi 7, I-67100 Laquila, Italy.
[Pettorino, V.] HGSFP, Philosophenweg 16, D-69120 Heidelberg, Germany.
[Pettorino, V.] Heidelberg Univ, Dept Theoret Phys, Philosophenweg 16, D-69120 Heidelberg, Germany.
[Partridge, B.] Haverford Coll, Dept Astron, 370 Lancaster Ave, Haverford, PA USA.
[Kurki-Suonio, H.; Lahteenmaki, A.; Savelainen, M.; Suur-Uski, A. -S.; Valiviita, J.] Univ Helsinki, Helsinki Inst Phys, Gustaf Hallstromin Katu 2, Helsinki 02540, Finland.
[Umana, G.] Osserv Astrofis Catania, INAF, Via S Sofia 78, I-95123 Catania, Italy.
[de Zotti, G.] Osserv Astron Padova, INAF, Vicolo Osserv 5, I-35131 Padua, Italy.
[Polenta, G.] Osserv Astron Roma, INAF, Via Frascati 33, I-00185 Rome, Italy.
[Frailis, M.; Galeotta, S.; Gregorio, A.; Maggio, G.; Maris, M.; Pasian, F.; Romelli, E.; Tavagnacco, D.; Vassallo, T.; Zacchei, A.] Osserv Astron Trieste, INAF, Via GB Tiepolo 11, I-43127 Trieste, Italy.
[Burigana, C.; Butler, R. C.; Cuttaia, F.; de Rosa, A.; Finelli, F.; Franceschi, E.; Gruppuso, A.; Mandolesi, N.; Morgante, G.; Natoli, P.; Paoletti, D.; Sandri, M.; Terenzi, L.; Toffolatti, L.; Valenziano, L.; Villa, F.] IASF Bologna, INAF, Via Gobetti 101, I-40127 Bologna, Italy.
[Bersanelli, M.; Donzelli, S.; Maino, D.; Mennella, A.; Rossetti, M.; Tomasi, M.] IASF Milano, INAF, Via E Bassini 15, I-20133 Milan, Italy.
[Burigana, C.; Finelli, F.; Paoletti, D.] Ist Nazl Fis Nucl, Sez Bologna, Via Irnerio 46, I-40126 Bologna, Italy.
[Melchiorri, A.; Pagano, L.] Univ Roma Sapienza, Ist Nazl Fis Nucl, Sez Roma 1, Piazzale Aldo Moro 2, I-00185 Rome, Italy.
[Renzi, A.] Univ Roma Tor Vergata, Ist Nazl Fis Nucl, Sez Roma 2, Via Ric Sci 1, I-00185 Rome, Italy.
[Gregorio, A.] Ist Nazl Fis Nucl, Natl Inst Nucl Phys, Via Valerio 2, I-34127 Trieste, Italy.
[Turler, M.] Univ Geneva, ISDC, Dept Astron, Ch Ecogia 16, CH-1290 Versoix, Switzerland.
[Mitra, S.] Pune Univ Campus, IUCAA, Post Bag 4, Pune 411007, Maharashtra, India.
[Ducout, A.; Jaffe, A. H.; Mortlock, D.] Imperial Coll London, Blackett Lab, Astrophys Grp, Prince Consort Rd, London SW7 2AZ, England.
[McGehee, P.; Pearson, T. J.; Rusholme, B.] CALTECH, Infrared Proc & Anal Ctr, Pasadena, CA 91125 USA.
[Benoit, A.] Univ Grenoble 1, CNRS, Inst Neel, 25 Rue Martyrs, F-38042 Grenoble, France.
[Dole, H.] Inst Univ France, 103 Bd St Michel, F-75005 Paris, France.
[Aghanim, N.; Aumont, J.; Chamballu, A.; Dole, H.; Douspis, M.; Hurier, G.; Kunz, M.; Lagache, G.; Mangilli, A.; Pajot, F.; Puget, J. -L.; Remazeilles, M.] Univ Paris 11, CNRS, Inst Astrophys Spatiale, UMR8617, Batiment 121, Orsay, France.
[Benabed, K.; Benoit-Levy, A.; Bouchet, F. R.; Cardoso, J. -F.; Colombi, S.; Ducout, A.; Elsner, F.; Hivon, E.; Prunet, S.; Sygnet, J. -F.; Wandelt, B. D.] CNRS, Inst Astrophys Paris, UMR7095, 98 Bis Blvd Arago, F-75014 Paris, France.
[Lesgourgues, J.] Rhein Westfal TH Aachen, Inst Theoret Teilchenphys & Kosmol, D-52056 Aachen, Germany.
[Efstathiou, G.; Gratton, S.; Harrison, D. L.; Migliaccio, M.; Sutton, D.] Univ Cambridge, Inst Astron, Madingley Rd, Cambridge CB3 0HA, England.
[Eriksen, H. K.; Gjerlow, E.; Hansen, F. K.; Lilje, P. B.; Wehus, I. K.] Univ Oslo, Inst Theoret Astrophys, N-0371 Oslo, Norway.
[Rebolo, R.; Rubino-Martin, J. A.] Inst Astrofis Canarias, C Via Lactea S-N, San Cristobal la Laguna 38200, Tenerife, Spain.
[Barreiro, R. B.; Bonavera, L.; Curto, A.; Diego, J. M.; Gonzalez-Nuevo, J.; Herranz, D.; Lopez-Caniego, M.; Martinez-Gonzalez, E.; Toffolatti, L.; Vielva, P.] Univ Cantabria, CSIC, Inst Fis Cantabria, Avda Castros S-N, Santander 39005, Spain.
[Bartolo, N.; Liguori, M.; Matarrese, S.] Ist Nazl Fis Nucl, Sez Padova, Via Marzolo 8, I-35131 Padua, Italy.
[Bock, J. J.; Colombo, L. P. L.; Crill, B. P.; Dore, O.; Gorski, K. M.; Hanson, D.; Hildebrandt, S. R.; Holmes, W. A.; Lawrence, C. R.; Mitra, S.; Pietrobon, D.; Prezeau, G.; Rocha, G.; Roudier, G.; Seiffert, M. D.; Wade, L. A.; Wehus, I. K.] CALTECH, Jet Prop Lab, 4800 Oak Grove Dr, Pasadena, CA USA.
[Bonaldi, A.; Davies, R. D.; Davis, R. J.; Dickinson, C.; Leahy, J. P.; Peel, M.; Remazeilles, M.; Watson, R.; Wilkinson, A.] Univ Manchester, Jodrell Bank Ctr Astrophys, Sch Phys & Astron, Alan Turing Bldg,Oxford Rd, Manchester M13 9PL, Lancs, England.
[Galli, S.] Univ Chicago, Kavli Inst Cosmol Phys, Chicago, IL 60637 USA.
[Ashdown, M.; Curto, A.; Gratton, S.; Harrison, D. L.; Lasenby, A.; Migliaccio, M.; Sutton, D.] Kavli Inst Cosmol Cambridge, Madingley Rd, Cambridge CB3 0HA, England.
[Stolyarov, V.] Kazan Fed Univ, 18 Kremlyovskaya St, Kazan 420008, Russia.
[Henrot-Versille, S.; Mangilli, A.; Perdereau, O.; Tristram, M.] Univ Paris 11, CNRS, IN2P3, LAL, Orsay, France.
[Catalano, A.; Lamarre, J. -M.; Levrier, F.; Roudier, G.] Observ Paris, CNRS, LERMA, 61 Ave Observ, F-75000 Paris, France.
[Chamballu, A.; Pratt, G. W.] Univ Paris Diderot, CEA DSM CNRS, CEA Saclay, IRFU,Serv Astrophys,ab AIM, Bat 709, F-91191 Gif Sur Yvette, France.
[Cardoso, J. -F.] CNRS, Lab Traitement & Commun Informat, UMR 5141, 46 Rue Barrault, F-75634 Paris 13, France.
[Cardoso, J. -F.] Telecom ParisTech, 46 Rue Barrault, F-75634 Paris 13, France.
[Catalano, A.; Macias-Perez, J. F.; Perotto, L.; Santos, D.] Univ Grenoble Alpes, CNRS, IN2P3, Lab Phys Subatom & Cosmol, 53 Rue Martyrs, F-38026 Grenoble, France.
[Van Tent, B.] Univ Paris 11, Phys Theor Lab, Batiment 210, F-91405 Orsay, France.
[Van Tent, B.] CNRS, Batiment 210, F-91405 Orsay, France.
[Kisner, T. S.] Lawrence Berkeley Natl Lab, Berkeley, CA USA.
[Novikov, D.; Novikov, I.] Russian Acad Sci, Ctr Astro Space, Lebedev Phys Inst, 84-32 Profsoyuznaya St,GSP-7, Moscow 117997, Russia.
[Ensslin, T. A.; Hovest, W.; Knoche, J.; Rachen, J. P.; Reinecke, M.] Max Planck Inst Astrophys, Karl Schwarzschild Str 1, D-85741 Garching, Germany.
[Hanson, D.] McGill Univ, McGill Phys, Ernest Rutherford Phys Bldg,3600 Rue Univ, Montreal, PQ H3A 2T8, Canada.
[Murphy, J. A.] Natl Univ Ireland, Dept Expt Phys, Maynooth, Kildare, Ireland.
[Bielewicz, P.] Nicolaus Copernicus Astron Ctr, Bartycka 18, PL-00716 Warsaw, Poland.
[Christensen, P. R.; Frejsel, A.; Novikov, I.] Niels Bohr Inst, Blegdamsvej 17, DK-1165 Copenhagen, Denmark.
[Naselsky, P.] Univ Copenhagen, Niels Bohr Inst, Blegdamsvej 17, DK-1165 Copenhagen, Denmark.
[Baccigalupi, C.; Bielewicz, P.; Danese, L.; de Zotti, G.; Paci, F.; Perrotta, F.] SISSA, Astrophys Sect, Via Bonomea 265, I-34136 Trieste, Italy.
[Terenzi, L.] Univ E Campus, SMARTEST Res Ctr, Via Isimbardi 10, I-22060 Novedrate, CO, Italy.
[Ade, P. A. R.; Munshi, D.; Spencer, L. D.] Cardiff Univ, Sch Phys & Astron, Queens Buildings, Cardiff CF24 3AA, S Glam, Wales.
[Moss, A.] Univ Nottingham, Sch Phys & Astron, Nottingham NG7 2RD, England.
[Bouchet, F. R.] UPMC, Sorbonne Univ, Inst Astrophys Paris, UMR7095, 98 Bis Blvd Arago, F-75014 Paris, France.
[Borrill, J.] Univ Calif Berkeley, Space Sci Lab, Berkeley, CA 94720 USA.
[Stolyarov, V.] Russian Acad Sci, Special Astrophys Observ, Nizhnii Arkhyz 369167, Zelenchukskiy R, Russia.
[Calabrese, E.] Univ Oxford, Subdept Astrophys, Keble Rd, Oxford OX1 3RH, England.
[Lesgourgues, J.] CERN, PH TH, Div Theory, CH-1211 Geneva 23, Switzerland.
[Benabed, K.; Benoit-Levy, A.; Colombi, S.; Elsner, F.; Hivon, E.; Prunet, S.; Wandelt, B. D.] Univ Paris 06, UMR7095, 98 Bis Blvd Arago, F-75014 Paris, France.
[Banday, A. J.; Bernard, J. -P.; Forni, O.; Giard, M.; Jaffe, T. R.; Montier, L.; Pointecouteau, E.] Univ Toulouse, UPS OMP, IRAP, F-31028 Toulouse 4, France.
[Battaner, E.] Univ Granada, Fac Ciencias, Dept Fis Teor & Cosmos, E-18071 Granada, Spain.
[Battaner, E.] Univ Granada, Inst Carlos Fis Teor & Computac 1, E-18071 Granada, Spain.
[Gorski, K. M.] Univ Warsaw Observ, Aleje Ujazdowskie 4, PL-00478 Warsaw, Poland.
RP Tomasi, M (reprint author), Univ Milan, Dipartimento Fis, Via Celoria 16, I-20133 Milan, Italy.; Tomasi, M (reprint author), IASF Milano, INAF, Via E Bassini 15, I-20133 Milan, Italy.
EM maurizio.tomasi@unimi.it
RI Herranz, Diego/K-9143-2014; Colombo, Loris/J-2415-2016; Lahteenmaki,
Anne/L-5987-2013; Barreiro, Rita Belen/N-5442-2014; bonavera,
laura/E-9368-2017; Gonzalez-Nuevo, Joaquin/I-3562-2014
OI Valiviita, Jussi/0000-0001-6225-3693; Hurier,
Guillaume/0000-0002-1215-0706; Toffolatti, Luigi/0000-0003-2645-7386;
Lilje, Per/0000-0003-4324-7794; Paoletti, Daniela/0000-0003-4761-6147;
Nati, Federico/0000-0002-8307-5088; Pierpaoli,
Elena/0000-0002-7957-8993; Juvela, Mika/0000-0002-5809-4834; Herranz,
Diego/0000-0003-4540-1417; Colombo, Loris/0000-0003-4572-7732;
Kurki-Suonio, Hannu/0000-0002-4618-3063; Zacchei,
Andrea/0000-0003-0396-1192; Stolyarov, Vladislav/0000-0001-8151-828X;
TERENZI, LUCA/0000-0001-9915-6379; Barreiro, Rita
Belen/0000-0002-6139-4272; bonavera, laura/0000-0001-8039-3876;
Gonzalez-Nuevo, Joaquin/0000-0003-1354-6822
FU ESA; CNES (France); CNRS/INSU-IN2P3-INP (France); ASI (Italy); CNR
(Italy); INAF (Italy); NASA (USA); DoE (USA); STFC (UK); UKSA (UK); CSIC
(Spain); MINECO (Spain); JA (Spain); RES (Spain); Tekes (Finland); AoF
(Finland); CSC (Finland); DLR (Germany); MPG (Germany); CSA (Canada);
DTU Space (Denmark); SER/SSO (Switzerland); RCN (Norway); SFI (Ireland);
FCT/MCTES (Portugal); ERC (EU); PRACE (EU)
FX The Planck Collaboration acknowledges the support of: ESA; CNES, and
CNRS/INSU-IN2P3-INP (France); ASI, CNR, and INAF (Italy); NASA and DoE
(USA); STFC and UKSA (UK); CSIC, MINECO, JA and RES (Spain); Tekes, AoF,
and CSC (Finland); DLR and MPG (Germany); CSA (Canada); DTU Space
(Denmark); SER/SSO (Switzerland); RCN (Norway); SFI (Ireland); FCT/MCTES
(Portugal); ERC and PRACE (EU). A description of the Planck
Collaboration and a list of its members, indicating which technical or
scientific activities they have been involved in, can be found at
http://www.cosmos.esa.int/web/planck/planck_collaboration
NR 45
TC 1
Z9 1
U1 0
U2 0
PU EDP SCIENCES S A
PI LES ULIS CEDEX A
PA 17, AVE DU HOGGAR, PA COURTABOEUF, BP 112, F-91944 LES ULIS CEDEX A,
FRANCE
SN 1432-0746
J9 ASTRON ASTROPHYS
JI Astron. Astrophys.
PD OCT
PY 2016
VL 594
AR A5
DI 10.1051/0004-6361/201526632
PG 24
WC Astronomy & Astrophysics
SC Astronomy & Astrophysics
GA DZ4MG
UT WOS:000385832200022
ER
PT J
AU Ade, PAR
Aghanim, N
Arnaud, M
Ashdown, M
Aumont, J
Baccigalupi, C
Banday, AJ
Barreiro, RB
Bartlett, JG
Bartolo, N
Battaner, E
Battye, R
Benabed, K
Benoit, A
Benoit-Levy, A
Bernard, JP
Bersanelli, M
Bielewicz, P
Bock, JJ
Bonaldi, A
Bonavera, L
Bond, JR
Borrinll, J
Bouchet, FR
Bucher, M
Burigana, C
Butler, RC
Calabrese, E
Cardoso, JF
Catalano, A
Challinor, A
Chamballu, A
Chary, RR
Chiang, HC
Christensen, PR
Church, S
Clements, DL
Colombi, S
Colombo, LPL
Combet, C
Comis, B
Couchot, F
Coulais, A
Crill, BP
Curto, A
Cuttaia, F
Danese, L
Davies, RD
Davis, RJ
de Bernardis, P
de Rosa, A
de Zotti, G
Delabrouille, J
Desert, FX
Diego, JM
Dolag, K
Dole, H
Donzelli, S
Dore, O
Douspis, M
Ducout, A
Dupac, X
Efstathiou, G
Elsner, F
Ensslin, TA
Eriksen, HK
Falgarone, E
Fergusson, J
Finelli, F
Forni, O
Frailis, M
Fraisse, AA
Franceschi, E
Frejsel, A
Galeotta, S
Galli, S
Ganga, K
Giard, M
Giraud-Heraud, Y
Gjerlow, E
Gonzalez-Nuevo, J
Gorski, KM
Gratton, S
Gregorio, A
Gruppuso, A
Gudmundsson, JE
Hansen, FK
Hanson, D
Harrison, DL
Henrot-Versille, S
Hernandez-Monteagudo, C
Herranz, D
Hildebrandt, SR
Hivon, E
Hobson, M
Holmes, WA
Hornstrup, A
Hovest, W
Huffenberger, KM
Hurier, G
Jaffe, AH
Jaffe, TR
Jones, WC
Juvela, M
Keihanen, E
Keskitalo, R
Kisner, TS
Kneissl, R
Knoche, J
Kunzo, M
Kurki-Suonio, H
Lagache, G
Lahteennmaki, A
Lamarre, JM
Lasenby, A
Lattanzi, M
Lawrence, CR
Leonardi, R
Lesgourgues, J
Levrier, F
Liguori, M
Lilje, PB
Linden-Vornle, M
Lopez-Caniego, M
Lubin, PM
Macias-Perez, JF
Maggio, G
Maino, D
Mandolesi, N
Mangilli, A
Maris, M
Martin, PG
Martinez-Gonzalez, E
Masi, S
Matarrese, S
McGehee, P
Meinhold, PR
Melchiorri', A
Melin, JB
Mendes, L
Mennella, A
Migliaccio, M
Mitrao, S
Miville-Deschenes, MA
Moneti, A
Montier, L
Morgante, G
Mortlock, D
Moss, A
Munshi, D
Murphy, JA
Naselsky, P
Nati, F
Natoli, P
Netterfield, CB
Norgaard-Nielsen, HU
Noviello, F
Novikov, D
Novikov, I
Oxborrow, CA
Paci, F
Pagano, L
Pajot, F
Paoletti, D
Partridge, B
Pasian, F
Patanchon, G
Pearson, TJ
Perdereau, O
Perotto, L
Perrotta, F
Pettorino, V
Piacentini, F
Piat, M
Pierpaoli, E
Pietrobon, D
Plaszczynski, S
Pointecouteau, E
Polenta, G
Popa, L
Prate, GW
Prezeau, G
Prunet, S
Puget, JL
Rachen, JP
Rebolo, R
Reinecke, M
Remazeilles, M
Renault, C
Renzi, A
Ristorcelli, I
Rocha, G
Roman, M
Rosset, C
Rossetti, M
Roudier, G
Rubino-Martin, JA
Rusholme, B
Sandri, M
Santos, D
Savelainen, M
Savini, G
Scott, D
Seiffert, MD
Shellard, EPS
Spencer, LD
Stolyarov, V
Stompor, R
Sudiwala, R
Sunyaev, R
Sutton, D
Suur-Uski, AS
Sygnet, JF
Tauber, JA
Terenzi, L
Toffolatti, L
Tomasi, M
Tristram, M
Tucci, M
Tuovinen, J
Turler, M
Umana, G
Valenziano, L
Valiviita', J
Van Tent, B
Vielva, P
Villa, F
Wade, LA
Wandelt, BD
Wehus, IK
Weller, J
White, SDM
Yvon, D
Zacchei, A
Zonca, A
AF Ade, P. A. R.
Aghanim, N.
Arnaud, M.
Ashdown, M.
Aumont, J.
Baccigalupi, C.
Banday, A. J.
Barreiro, R. B.
Bartlett, J. G.
Bartolo, N.
Battaner, E.
Battye, R.
Benabed, K.
Benoit, A.
Benoit-Levy, A.
Bernard, J. -P.
Bersanelli, M.
Bielewicz, P.
Bock, J. J.
Bonaldi, A.
Bonavera, L.
Bond, J. R.
Borrinll, J.
Bouchet, F. R.
Bucher, M.
Burigana, C.
Butler, R. C.
Calabrese, E.
Cardoso, J. -F.
Catalano, A.
Challinor, A.
Chamballu, A.
Chary, R. -R.
Chiang, H. C.
Christensen, P. R.
Church, S.
Clements, D. L.
Colombi, S.
Colombo, L. P. L.
Combet, C.
Comis, B.
Couchot, F.
Coulais, A.
Crill, B. P.
Curto, A.
Cuttaia, F.
Danese, L.
Davies, R. D.
Davis, R. J.
de Bernardis, P.
de Rosa, A.
de Zotti, G.
Delabrouille, J.
Desert, F. -X.
Diego, J. M.
Dolag, K.
Dole, H.
Donzelli, S.
Dore, O.
Douspis, M.
Ducout, A.
Dupac, X.
Efstathiou, G.
Elsner, F.
Ensslin, T. A.
Eriksen, H. K.
Falgarone, E.
Fergusson, J.
Finelli, F.
Forni, O.
Frailis, M.
Fraisse, A. A.
Franceschi, E.
Frejsel, A.
Galeotta, S.
Galli, S.
Ganga, K.
Giard, M.
Giraud-Heraud, Y.
Gjerlow, E.
Gonzalez-Nuevo, J.
Gorski, K. M.
Gratton, S.
Gregorio, A.
Gruppuso, A.
Gudmundsson, J. E.
Hansen, F. K.
Hanson, D.
Harrison, D. L.
Henrot-Versille, S.
Hernandez-Monteagudo, C.
Herranz, D.
Hildebrandt, S. R.
Hivon, E.
Hobson, M.
Holmes, W. A.
Hornstrup, A.
Hovest, W.
Huffenberger, K. M.
Hurier, G.
Jaffe, A. H.
Jaffe, T. R.
Jones, W. C.
Juvela, M.
Keihanen, E.
Keskitalo, R.
Kisner, T. S.
Kneissl, R.
Knoche, J.
Kunzo, M.
Kurki-Suonio, H.
Lagache, G.
Lahteennmaki, A.
Lamarre, J. -M.
Lasenby, A.
Lattanzi, M.
Lawrence, C. R.
Leonardi, R.
Lesgourgues, J.
Levrier, F.
Liguori, M.
Lilje, P. B.
Linden-Vornle, M.
Lopez-Caniego, M.
Lubin, P. M.
Macias-Perez, J. F.
Maggio, G.
Maino, D.
Mandolesi, N.
Mangilli, A.
Maris, M.
Martin, P. G.
Martinez-Gonzalez, E.
Masi, S.
Matarrese, S.
McGehee, P.
Meinhold, P. R.
Melchiorri', A.
Melin, J. -B.
Mendes, L.
Mennella, A.
Migliaccio, M.
Mitrao, S.
Miville-Deschenes, M. -A.
Moneti, A.
Montier, L.
Morgante, G.
Mortlock, D.
Moss, A.
Munshi, D.
Murphy, J. A.
Naselsky, P.
Nati, F.
Natoli, P.
Netterfield, C. B.
Norgaard-Nielsen, H. U.
Noviello, F.
Novikov, D.
Novikov, I.
Oxborrow, C. A.
Paci, F.
Pagano, L.
Pajot, F.
Paoletti, D.
Partridge, B.
Pasian, F.
Patanchon, G.
Pearson, T. J.
Perdereau, O.
Perotto, L.
Perrotta, F.
Pettorino, V.
Piacentini, F.
Piat, M.
Pierpaoli, E.
Pietrobon, D.
Plaszczynski, S.
Pointecouteau, E.
Polenta, G.
Popa, L.
Prate, G. W.
Prezeau, G.
Prunet, S.
Puget, J. -L.
Rachen, J. P.
Rebolo, R.
Reinecke, M.
Remazeilles, M.
Renault, C.
Renzi, A.
Ristorcelli, I.
Rocha, G.
Roman, M.
Rosset, C.
Rossetti, M.
Roudier, G.
Rubino-Martin, J. A.
Rusholme, B.
Sandri, M.
Santos, D.
Savelainen, M.
Savini, G.
Scott, D.
Seiffert, M. D.
Shellard, E. P. S.
Spencer, L. D.
Stolyarov, V.
Stompor, R.
Sudiwala, R.
Sunyaev, R.
Sutton, D.
Suur-Uski, A. -S.
Sygnet, J. -F.
Tauber, J. A.
Terenzi, L.
Toffolatti, L.
Tomasi, M.
Tristram, M.
Tucci, M.
Tuovinen, J.
Turler, M.
Umana, G.
Valenziano, L.
Valiviita', J.
Van Tent, B.
Vielva, P.
Villa, F.
Wade, L. A.
Wandelt, B. D.
Wehus, I. K.
Weller, J.
White, S. D. M.
Yvon, D.
Zacchei, A.
Zonca, A.
CA Planck Collaboration
TI Planck 2015 results XXIV. Cosmology from Sunyaev-Zeldovich cluster
counts
SO ASTRONOMY & ASTROPHYSICS
LA English
DT Article
DE cosmological parameters; large-scale structure of Universe
ID BARYON ACOUSTIC-OSCILLATIONS; SOUTH-POLE TELESCOPE; HALO MASS FUNCTION;
LOCAL GALAXY CLUSTERS; WEAK-LENSING MASSES; X-RAY; INTRACLUSTER MEDIUM;
SCALING RELATIONS; PRECISION COSMOLOGY; HUBBLE CONSTANT
AB We present cluster counts and corresponding cosmological constraints from the Planck full mission data set. Our catalogue consists of 439 clusters detected via their Sunyaev-Zeldovich (SZ) signal down to a signal-to-noise ratio of 6, and is more than a factor of 2 larger than the 2013 Planck cluster cosmology sample. The counts are consistent with those from 2013 and yield compatible constraints under the same modelling assumptions. Taking advantage of the larger catalogue, we extend our analysis to the two-dimensional distribution in redshift and signal-to-noise. We use mass estimates from two recent studies of gravitational lensing of background galaxies by Planck clusters to provide priors on the hydrostatic bias parameter, (1 - b). In addition, we use lensing of cosmic microwave background (CMB) temperature fluctuations by Planck clusters as an independent constraint on this parameter. These various calibrations imply constraints on the present-day amplitude of matter fluctuations in varying degrees of tension with those from the Planck analysis of primary fluctuations in the CMB; for the lowest estimated values of (1 b) the tension is mild, only a little over one standard deviation, while it remains substantial (3.7 sigma) for the largest estimated value. We also examine constraints on extensions to the base flat Lambda CDM model by combining the cluster and CMB constraints. The combination appears to favour non-minimal neutrino masses, but this possibility does little to relieve the overall tension because it simultaneously lowers the implied value of the Hubble parameter, thereby exacerbating the discrepancy with most current astrophysical estimates. Improving the precision of cluster mass calibrations from the current 10%-level to 1% would significantly strengthen these combined analyses and provide a stringent test of the base Lambda CDM model.
C1 [Bartlett, J. G.; Bucher, M.; Delabrouille, J.; Ganga, K.; Giraud-Heraud, Y.; Patanchon, G.; Piat, M.; Remazeilles, M.; Roman, M.; Rosset, C.; Roudier, G.; Stompor, R.] Univ Paris Diderot, APC, CNRS IN2P3, CEA Lrfu,Observ Paris,Sorbonne Paris Cite, 10 Rue Alice Domon & Leonie Duquet, F-75205 Paris 13, France.
[Lahteennmaki, A.] Aalto Univ, Metsahovi Radio Observ, POB 13000, Aalto 00076, Finland.
[Lahteennmaki, A.] Aalto Univ, Dept Radio Sci & Engn, POB 13000, Aalto 00076, Finland.
[Bartolo, N.; Kunzo, M.] African Inst Math Sci, 6-8 Melrose Rd, ZA-7945 Cape Town, South Africa.
[Natoli, P.; Polenta, G.] Agenzia Spaziale Italiana, Sci Data Ctr, Via Politecn Snc, I-00133 Rome, Italy.
[Lagache, G.] Aix Marseille Univ, CNRS, LAM, UMR 7326, F-13388 Marseille, France.
[Ashdown, M.; Curto, A.; Hobson, M.; Lasenby, A.; Stolyarov, V.] Univ Cambridge, Cavendish Lab, Astrophys Grp, JJ Thomson Ave, Cambridge CB3 0HE, England.
[Chiang, H. C.] Univ KwaZulu Natal, Sch Math Stat & Comp Sci, Astrophys & Cosmol Res Unit, Westville Campus,Private Bag X54001, ZA-4000 Durban, South Africa.
[Kneissl, R.] ALMA Santiago Cent Off, Atacama Large Millimeter Submillimeter Array, Alonso Cordova 3107,763 0355 Casilla, Santiago, Chile.
[Leonardi, R.] CGEE, SCS Qd 9,Lote C,Torre C,4 Andar, BR-70308200 Brasilia, DF, Brazil.
[Bond, J. R.; Hanson, D.; Martin, P. G.; Miville-Deschenes, M. -A.] Univ Toronto, CITA, 60 St George St, Toronto, ON M5S 3H8, Canada.
[Banday, A. J.; Bernard, J. -P.; Bielewicz, P.; Cardoso, J. -F.; Forni, O.; Giard, M.; Jaffe, T. R.; Montier, L.; Pointecouteau, E.; Ristorcelli, I.] IRAP, CNRS, 9 Ave Colonel Roche,BP 44346, F-31028 Toulouse 4, France.
[Tuovinen, J.] Trinity Coll Dublin, CRANN, Dublin, Ireland.
[Bock, J. J.; Crill, B. P.; Dore, O.; Hildebrandt, S. R.; Pearson, T. J.; Prezeau, G.; Rocha, G.; Seiffert, M. D.] CALTECH, Pasadena, CA 91125 USA.
[Challinor, A.; Fergusson, J.; Shellard, E. P. S.] Univ Cambridge, DAMTP, Ctr Theoret Cosmol, Wilberforce Rd, Cambridge CB3 0WA, England.
[Hernandez-Monteagudo, C.] CEFCA, Plaza San Juan 1,Planta 2, Teruel 44001, Spain.
[Borrinll, J.; Keskitalo, R.] Lawrence Berkeley Natl Lab, Computat Cosmol Ctr, Berkeley, CA 94720 USA.
[Rebolo, R.] CSIC, Madrid 28006, Spain.
[Chamballu, A.; Melin, J. -B.; Yvon, D.] CEA Saclay, DSM Irfu SPP, F-91191 Gif Sur Yvette, France.
[Hornstrup, A.; Linden-Vornle, M.; Norgaard-Nielsen, H. U.; Oxborrow, C. A.] Tech Univ Denmark, Natl Space Inst, DTU Space, Elektrovej 327, DK-2800 Lyngby, Denmark.
[Kunzo, M.; Tucci, M.] Univ Geneva, Dept Phys Theor, 24 Quai E Ansermet, CH-1211 Geneva 4, Switzerland.
[Rebolo, R.; Rubino-Martin, J. A.] Univ La Laguna, Dept Astrofis, E-38206 Tenerife, Spain.
[Gonzalez-Nuevo, J.; Toffolatti, L.] Univ Oviedo, Dept Fis, Avda Calvo Sotelo S-N, Oviedo 33007, Spain.
[Netterfield, C. B.] Univ Toronto, Dept Astron & Astrophys, 50 St George St,38100, Toronto, ON, Canada.
[Rachen, J. P.] Radboud Univ Nijmegen, Dept Astrophys IMAPP, POB 9010, NL-6500 GL Nijmegen, Netherlands.
[Scott, D.] Univ British Columbia, Dept Phys & Astron, 6224 Agr Rd, Vancouver, BC, Canada.
[Colombo, L. P. L.; Pierpaoli, E.] Univ Southern Calif, Dana & David Dornsife Coll Letter Arts & Sci, Dept Phys & Astron, Los Angeles, CA 90089 USA.
[Benoit-Levy, A.; Elsner, F.] UCL, Dept Phys & Astron, London WC1E 6BT, England.
[Huffenberger, K. M.] Florida State Univ, Dept Phys, Keen Phys Bldg,77 Chieftan Way, Tallahassee, FL 32306 USA.
[Juvela, M.; Keihanen, E.; Kurki-Suonio, H.; Savelainen, M.; Suur-Uski, A. -S.; Valiviita', J.] Univ Helsinki, Dept Phys, Gustaf Hallstromin Katu 2a, Helsinki 00014, Finland.
[Chiang, H. C.; Fraisse, A. A.; Gudmundsson, J. E.; Jones, W. C.; Nati, F.] Princeton Univ, Dept Phys, Princeton, NJ 08544 USA.
[Lubin, P. M.; Meinhold, P. R.; Zonca, A.] Univ Calif Santa Barbara, Dept Phys, Santa Barbara, CA 93106 USA.
[Wandelt, B. D.] Univ Illinois, Dept Phys, 1110 West Green St, Urbana, IL 61801 USA.
[Liguori, M.; Matarrese, S.] Univ Padua, Dipartimento Fis & Astron G Galilei, Via Marzolo 8, I-35131 Padua, Italy.
[Burigana, C.; Lattanzi, M.; Mandolesi, N.; Natoli, P.] Univ Ferrara, Dipartimento Fis & Sci Terra, Via Saragat 1, I-44122 Ferrara, Italy.
[de Bernardis, P.; Masi, S.; Melchiorri', A.; Pagano, L.; Piacentini, F.] Univ Roma La Sapienza, Dipartimento Fis, Ple A Moro 2, I-00133 Rome, Italy.
[Bersanelli, M.; Maino, D.; Mennella, A.; Rossetti, M.; Tomasi, M.] Univ Milan, Dipartimento Fis, Via Celoria 16, I-20133 Milan, Italy.
[Gregorio, A.] Univ Trieste, Dipartimento Fis, Via A Valerio 2, I-34127 Trieste, Italy.
[Renzi, A.] Univ Roma Tor Vergata, Dipartimento Matemat, Via Ric Sci 1, I-00133 Rome, Italy.
[Christensen, P. R.] Niels Bohr Inst, Discovery Ctr, Blegdamsvej 17, Copenhagen, Denmark.
[Naselsky, P.] Univ Copenhagen, Niels Bohr Inst, Discovery Ctr, Blegdamsvej 17, DK-1165 Copenhagen, Denmark.
[Kneissl, R.] European Southern Observ, ESO Vitacura, Alonso Cordova 3107,Casilla 19001, Santiago, Chile.
[Dupac, X.; Lopez-Caniego, M.; Mendes, L.] European Space Agcy, ESAC, Planck Sci Off, Camino Bajo Castillo S-N, Madrid, Spain.
[Tauber, J. A.] European Space Agcy, Estec, Keplerlaan 1, NL-2201 AZ Noordwijk, Netherlands.
[Matarrese, S.] Ist Nazl Fis Nucl, Gran Sasso Sci Inst, Viale F Crispi 7, I-67100 Laquila, Italy.
[Pettorino, V.] HGSFP, Philosophenweg 16, D-69120 Heidelberg, Germany.
[Pettorino, V.] Heidelberg Univ, Dept Theoret Phys, Philosophenweg 16, D-69120 Heidelberg, Germany.
[Partridge, B.] Haverford Coll, Dept Astron, 370 Lancaster Ave, Haverford, PA USA.
[Kurki-Suonio, H.; Lahteennmaki, A.; Savelainen, M.; Suur-Uski, A. -S.; Valiviita', J.] Univ Helsinki, Helsinki Inst Phys, Gustaf Hallstromin Katu 2, Helsinki 00560, Finland.
[Umana, G.] INAF Osservatorio Astrofis Catania, Via S Sofia 78, Catania, Italy.
[de Zotti, G.] INAF Osservatorio Astron Padova, Vicolo Osservatorio 5, I-35131 Padua, Italy.
[Polenta, G.] INAF Osservatorio Astron Roma, Via Frascati 33, I-00040 Monte Porzio Catone, Italy.
[Frailis, M.; Galeotta, S.; Gregorio, A.; Maggio, G.; Maris, M.; Pasian, F.; Zacchei, A.] INAF Osservatorio Astron Trieste, Via GB Tiepolo 11, I-40127 Trieste, Italy.
[Burigana, C.; Butler, R. C.; Cuttaia, F.; de Rosa, A.; Finelli, F.; Franceschi, E.; Gruppuso, A.; Mandolesi, N.; Morgante, G.; Natoli, P.; Paoletti, D.; Sandri, M.; Terenzi, L.; Toffolatti, L.; Valenziano, L.; Villa, F.] INAF IASF Bologna, Via Gobetti 101, I-40129 Bologna, Italy.
[Bersanelli, M.; Donzelli, S.; Maino, D.; Mennella, A.; Rossetti, M.; Tomasi, M.] INAF IASF Milano, Via E Bassini 15, I-20133 Milan, Italy.
[Burigana, C.; Finelli, F.] Ist Nazl Fis Nucl, Sez Bologna, Via Irnerio 46, I-40126 Bologna, Italy.
[Melchiorri', A.; Pagano, L.] Univ Roma Sapienza, Sez Roma 1, Ist Nazl Fis Nucl, Piazzale Aldo Moro 2, I-00185 Rome, Italy.
[Renzi, A.] Univ Roma Tor Vergata, Sez Roma 2, Ist Nazl Fis Nucl, Via Ric Sci 1, I-00185 Rome, Italy.
[Gregorio, A.] INFN Natl Inst Nucl Phys, Via Valerio 2, I-34127 Trieste, Italy.
[Desert, F. -X.] Univ Grenoble Alpes, IPAG, CNRS, F-38000 Grenoble, France.
[Turler, M.] Univ Geneva, Dept Astron, ISDC, Ch Ecogia 16, CH-1290 Versoix, Switzerland.
[Mitrao, S.] IUCAA, Post Bag 4,Pune Univ Campus, Pune 411007, Maharashtra, India.
[Clements, D. L.; Ducout, A.; Jaffe, A. H.; Mortlock, D.] Imperial Coll London, Astrophys Grp, Blackett Lab, Prince Consort Rd, London SW7 2AZ, England.
[Chary, R. -R.; McGehee, P.; Pearson, T. J.; Rusholme, B.] CALTECH, Infrared Proc & Anal Ctr, Pasadena, CA 91125 USA.
[Benoit, A.] Univ Joseph Fourier Grenoble I, CNRS, Inst Neel, 25 Rue Martyrs, Grenoble, France.
[Dole, H.] Inst Univ France, 103 Bd St Michel, F-75005 Paris, France.
[Aghanim, N.; Aumont, J.; Chamballu, A.; Dole, H.; Douspis, M.; Hurier, G.; Kunzo, M.; Lagache, G.; Mangilli, A.; Miville-Deschenes, M. -A.; Pajot, F.; Puget, J. -L.; Remazeilles, M.] Univ Paris Saclay, CNRS, Inst Astrophys Spatiale, Bat 121, F-91405 Orsay, France.
[Benabed, K.; Benoit-Levy, A.; Bouchet, F. R.; Cardoso, J. -F.; Colombi, S.; Ducout, A.; Elsner, F.; Hivon, E.; Migliaccio, M.; Moneti, A.; Prunet, S.; Sygnet, J. -F.; Wandelt, B. D.] CNRS, Inst Astrophys Paris, UMR7095, 98bis Blvd Arago, F-75014 Paris, France.
[Lesgourgues, J.] Rhein Westfal TH Aachen, Inst Theoret Teilchenphys & Kosmol, D-52056 Aachen, Germany.
[Popa, L.] Inst Space Sci, Bucharest, Romania.
[Challinor, A.; Efstathiou, G.; Gratton, S.; Harrison, D. L.; Sutton, D.] Univ Cambridge, Inst Astron, Madingley Rd, Cambridge CB3 0HA, England.
[Eriksen, H. K.; Gjerlow, E.; Hansen, F. K.; Lilje, P. B.; Wehus, I. K.] Univ Oslo, Inst Theoret Astrophys, N-0371 Oslo, Norway.
[Rebolo, R.; Rubino-Martin, J. A.] Inst Astrofis Canarias, C Via Lactea S-N, Tenerife 38205, Spain.
[Barreiro, R. B.; Bonavera, L.; Curto, A.; Diego, J. M.; Gonzalez-Nuevo, J.; Herranz, D.; Lopez-Caniego, M.; Martinez-Gonzalez, E.; Toffolatti, L.; Vielva, P.] Univ Cantabria, CSIC, Inst Fis Cantabria, Avda Castros S-N, Santander 39005, Spain.
[Bartolo, N.; Liguori, M.; Matarrese, S.] Ist Nazl Fis Nucl, Sez Padova, Via Marzolo 8, I-35131 Padua, Italy.
[Bartlett, J. G.; Colombo, L. P. L.; Crill, B. P.; Dore, O.; Gorski, K. M.; Hanson, D.; Hildebrandt, S. R.; Holmes, W. A.; Lawrence, C. R.; Mitrao, S.; Pietrobon, D.; Prezeau, G.; Rocha, G.; Roudier, G.; Seiffert, M. D.; Wade, L. A.; Wehus, I. K.] CALTECH, Jet Prop Lab, 4800 Oak Grove Dr, Pasadena, CA USA.
[Battye, R.; Bock, J. J.; Bonaldi, A.; Davies, R. D.; Davis, R. J.; Noviello, F.; Remazeilles, M.] Univ Manchester, Sch Phys & Astron, Jodrell Bank Ctr Astrophys, Alan Turing Bldg,Oxford Rd, Manchester M13 9PL, Lancs, England.
[Galli, S.] Univ Chicago, Kavli Inst Cosmol Phys, Chicago, IL 60637 USA.
[Ashdown, M.; Challinor, A.; Curto, A.; Gratton, S.; Harrison, D. L.; Lasenby, A.; Migliaccio, M.; Sutton, D.] Kavli Inst Cosmol Cambridge, Madingley Rd, Cambridge CB3 0HA, England.
[Stolyarov, V.] Kazan Fed Univ, 18 Kremlyovskaya St, Kazan 420008, Russia.
[Couchot, F.; Henrot-Versille, S.; Mangilli, A.; Perdereau, O.; Plaszczynski, S.; Tristram, M.] Univ Paris 11, LAL, CNRS IN2P3, F-91898 Orsay, France.
[Catalano, A.; Coulais, A.; Falgarone, E.; Lamarre, J. -M.; Levrier, F.; Roudier, G.] Observ Paris, CNRS, LERMA, 61 Ave Observ, F-75000 Paris, France.
[Arnaud, M.; Chamballu, A.; Prate, G. W.] Univ Paris Diderot, CEA DSM, IRFU Serv Astrophys, Lab AIM,CNRS, Bat 709, F-91191 Gif Sur Yvette, France.
[Cardoso, J. -F.] CNRS, Lab Traitement & Commun Informat, UMR 5141, 46 Rue Barrault, F-75634 Paris 13, France.
[Cardoso, J. -F.] Telecom ParisTech, 46 Rue Barrault, F-75634 Paris 13, France.
[Catalano, A.; Combet, C.; Comis, B.; Macias-Perez, J. F.; Perotto, L.; Renault, C.; Santos, D.] Univ Grenoble Alpes, Lab Phys Subat & Cosmol, CNRS IN2P3, 53 Rue Martyrs, F-38026 Grenoble, France.
[Van Tent, B.] Univ Paris Sud 11, Lab Phys Theor, Batiment 210, F-91405 Orsay, France.
[Van Tent, B.] CNRS, Batiment 210, F-91405 Orsay, France.
[Kisner, T. S.] Lawrence Berkeley Natl Lab, Berkeley, CA USA.
[Novikov, D.; Novikov, I.] Russian Acad Sci, Lebedev Phys Inst, Ctr Astro Space, 84-32 Profsoyuznaya St,GS7, Moscow 117997, Russia.
[Dolag, K.; Ensslin, T. A.; Hernandez-Monteagudo, C.; Hovest, W.; Knoche, J.; Rachen, J. P.; Reinecke, M.; Sunyaev, R.; White, S. D. M.] Max Planck Inst Astrophys, Karl Schwarzschild Str 1, D-85741 Garching, Germany.
[Hanson, D.] McGill Univ, McGill Phys, Ernest Rutherford Phys Bldg,3600 Rue Univ, Montreal, PQ H3A 2T8, Canada.
[Murphy, J. A.] Natl Univ Ireland, Dept Expt Phys, Maynooth, Kildare, Ireland.
[Bielewicz, P.] Nicolaus Copernicus Astron Ctr, Bartycka 18, PL-00716 Warsaw, Poland.
[Christensen, P. R.; Frejsel, A.; Novikov, I.] Niels Bohr Inst, Blegdamsvej 17, DK-1165 Copenhagen, Denmark.
[Naselsky, P.] Univ Copenhagen, Niels Bohr Inst, Blegdamsvej 17, DK-1165 Copenhagen, Denmark.
[Gudmundsson, J. E.] Nordita Nord Inst Theoret Phys, Roslagstullsbacken 23, S-10691 Stockholm, Sweden.
[Savini, G.] UCL, Opt Sci Lab, Gower St, London, England.
[Baccigalupi, C.; Bielewicz, P.; de Zotti, G.; Paci, F.; Perrotta, F.] SISSA, Astrophys Sect, Via Bonomea 265, I-34136 Trieste, Italy.
[Terenzi, L.] Univ E Campus, SMARTEST Res Ctr, Via Isimbardi 10, I-22060 Novedrate, CO, Italy.
[Ade, P. A. R.; Danese, L.; Munshi, D.; Spencer, L. D.; Sudiwala, R.] Cardiff Univ, Sch Phys & Astron, Queens Bldg, Cardiff CF24 3AA, S Glam, Wales.
[Moss, A.] Univ Nottingham, Sch Phys & Astron, Nottingham NG7 2RD, England.
[Bouchet, F. R.] Sorbonne Univ UPMC, UMR7095, Inst Astrophys Paris, 98bis Blvd Arago, F-75014 Paris, France.
[Sunyaev, R.] Russian Acad Sci, Space Res Inst IKI, Profsoyuznaya Str 84-32, Moscow 117997, Russia.
[Borrinll, J.] Univ Calif Berkeley, Space Sci Lab, Berkeley, CA 94720 USA.
[Stolyarov, V.] Russian Acad Sci, Special Astrophys Observ, Karachai Cherkessian Rep 369167, Zelenchukskiy R, Russia.
[Church, S.] Stanford Univ, Dept Phys, Varian Phys Bldg,382 Via Pueblo Mall, Stanford, CA USA.
[Calabrese, E.] Univ Oxford, Subdept Astrophys, Oxford OX1 3RH, England.
[Gudmundsson, J. E.] Stockholm Univ, Oskar Klein Ctr Cosmoparticle Phys, Dept Phys, AlbaNova, S-10691 Stockholm, Sweden.
[Lesgourgues, J.] CERN, PH TH, Div Theory, CH-1211 Geneva 23, Switzerland.
[Benabed, K.; Benoit-Levy, A.; Colombi, S.; Elsner, F.; Hivon, E.; Prunet, S.; Wandelt, B. D.] UPMC Univ Paris 06, UMR7095, 98bis Blvd Arago, F-75014 Paris, France.
[Banday, A. J.; Bernard, J. -P.; Forni, O.; Giard, M.; Jaffe, T. R.; Montier, L.; Pointecouteau, E.; Ristorcelli, I.] Univ Toulouse, UPS OMP, IRAP, F-31028 Toulouse 4, France.
[Dolag, K.; Weller, J.] Ludwig Maximilian Univ Munich, Univ Observ, Scheinerstr 1, D-81679 Munich, Germany.
[Battaner, E.] Univ Granada, Dept Fis Teor & Cosmos, Fac Ciencias, Granada 81679, Spain.
[Battaner, E.] Univ Granada, Inst Carlos Fis Teor & Computac 1, Granada, Spain.
[Gorski, K. M.] Univ Warsaw Observ, Aleje Ujazdowskie 4, PL-00478 Warsaw, Poland.
RP Bonaldi, A (reprint author), Univ Manchester, Sch Phys & Astron, Jodrell Bank Ctr Astrophys, Alan Turing Bldg,Oxford Rd, Manchester M13 9PL, Lancs, England.
EM anna.bonaldi@manchester.ac.uk
RI bonavera, laura/E-9368-2017; Gonzalez-Nuevo, Joaquin/I-3562-2014;
Herranz, Diego/K-9143-2014; Colombo, Loris/J-2415-2016; Barreiro, Rita
Belen/N-5442-2014
OI Hivon, Eric/0000-0003-1880-2733; Toffolatti, Luigi/0000-0003-2645-7386;
Lilje, Per/0000-0003-4324-7794; Paoletti, Daniela/0000-0003-4761-6147;
Nati, Federico/0000-0002-8307-5088; Savini, Giorgio/0000-0003-4449-9416;
Pierpaoli, Elena/0000-0002-7957-8993; Juvela, Mika/0000-0002-5809-4834;
bonavera, laura/0000-0001-8039-3876; Gonzalez-Nuevo,
Joaquin/0000-0003-1354-6822; Herranz, Diego/0000-0003-4540-1417;
Colombo, Loris/0000-0003-4572-7732; TERENZI, LUCA/0000-0001-9915-6379;
Stolyarov, Vladislav/0000-0001-8151-828X; Valiviita,
Jussi/0000-0001-6225-3693; Hurier, Guillaume/0000-0002-1215-0706;
Kurki-Suonio, Hannu/0000-0002-4618-3063; Zacchei,
Andrea/0000-0003-0396-1192; Barreiro, Rita Belen/0000-0002-6139-4272
FU ESA; CNES (France); CNRS/INSU-IN2P3-INP (France); ASI (Italy); CNR
(Italy); INAF (Italy); NASA (USA); DoE (USA); STFC (UK); UKSA (UK); CSIC
(Spain); MINECO (Spain); JA (Spain); RES (Spain); Tekes (Finland); AoF
(Finland); CSC (Finland); DLR (Germany); MPG (Germany); CSA (Canada);
DTU Space (Denmark); SER/SSO (Switzerland); RCN (Norway); SFI (Ireland);
FCT/MCTES (Portugal); ERC (EU); PRACE (EU)
FX The Planck Collaboration acknowledges the support of: ESA; CNES, and
CNRS/INSU-IN2P3-INP (France); ASI, CNR, and INAF (Italy); NASA and DoE
(USA); STFC and UKSA (UK); CSIC, MINECO, JA and RES (Spain); Tekes, AoF,
and CSC (Finland); DLR and MPG (Germany); CSA (Canada); DTU Space
(Denmark); SER/SSO (Switzerland); RCN (Norway); SFI (Ireland); FCT/MCTES
(Portugal); ERC and PRACE (EU). A description of the Planck
Collaboration and a list of its members, indicating which technical or
scientific activities they have been involved in, can be found at
http://www.cosmos.esa.int/web/planck/planck-collaboration.
NR 103
TC 3
Z9 3
U1 1
U2 1
PU EDP SCIENCES S A
PI LES ULIS CEDEX A
PA 17, AVE DU HOGGAR, PA COURTABOEUF, BP 112, F-91944 LES ULIS CEDEX A,
FRANCE
SN 1432-0746
J9 ASTRON ASTROPHYS
JI Astron. Astrophys.
PD OCT
PY 2016
VL 594
AR A24
DI 10.1051/0004-6361/201525833
PG 19
WC Astronomy & Astrophysics
SC Astronomy & Astrophysics
GA DZ4MG
UT WOS:000385832200015
ER
PT J
AU Ade, PAR
Aghanim, N
Arnaud, M
Ashdown, M
Aumont, J
Baccigalupi, C
Banday, AJ
Barreiro, RB
Bartolo, N
Basak, S
Battaner, E
Benabed, K
Benoit, A
Benoit-Levy, A
Bernard, JP
Bersanelli, M
Bielewicz, P
Bock, JJ
Bonaldi, A
Bonavera, L
Bond, JR
Borrill, J
Bouchet, FR
Bucher, M
Burigana, C
Butler, RC
Calabrese, E
Cardoso, JF
Catalano, A
Challinor, A
Chamballu, A
Chiang, HC
Christensen, PR
Church, S
Clements, DL
Colombi, S
Colombo, LPL
Combet, C
Couchot, F
Coulais, A
Crill, BP
Curto, A
Cuttaia, F
Danese, L
Davies, RD
Davis, RJ
de Bernardis, P
de Rosa, A
de Zotti, G
Delabrouille, J
Desert, FX
Diego, JM
Dole, H
Donzelli, S
Dore, O
Douspis, M
Ducout, A
Dupac, X
Efstathiou, G
Elsner, F
Ensslin, TA
Eriksen, HK
Feeney, S
Fergusson, J
Finelli, F
Forni, O
Frailis, M
Fraisse, AA
Franceschi, E
Frejse, A
Galeotta, S
Galli, S
Ganga, K
Giard, M
Giraud-Heraud, Y
Gjerlow, E
Gonzalez-Nuevo, J
Gorski, KM
Gratton, S
Gregorio, A
Gruppuso, A
Gudmundsson, JE
Hansen, FK
Hanson, D
Harrison, DL
Henrot-Versille, S
Hernandez-Monteagudo, C
Herranz, D
Hildebrandt, SR
Hivon, E
Hobson, M
Holmes, WA
Hornstrup, A
Hovest, W
Huffenberger, KM
Hurier, G
Jaffe, AH
Jaffe, TR
Jones, WC
Juvela, M
Keihanen, E
Keskitalo, R
Kisner, TS
Knoche, J
Kunz, M
Kurki-Suonio, H
Lagache, G
Lahteenmaki, A
Lamarre, JM
Lasenby, A
Lattanzi, M
Lawrence, CR
Leonardi, R
Lesgourgues, J
Levrier, F
Liguori, M
Lilje, PB
Linden-Vornle, M
Lopez-Caniego, M
Lubin, PM
Macias-Perez, JF
Maggio, G
Maino, D
Mandolesi, N
Mangilli, A
Maris, M
Martin, PG
Martinez-Gonzalez, E
Masi, S
Matarrese, S
McEwen, JD
McGehee, P
Meinhold, PR
Melchiorri, A
Mendes, L
Mennella, A
Migliaccio, M
Mitra, S
Miville-Deschenes, MA
Moneti, A
Montier, L
Morgante, G
Mortlock, D
Moss, A
Munshi, D
Murphy, JA
Naselsky, P
Nati, F
Natoli, P
Netterfield, CB
Norgaard-Nielsen, HU
Noviello, F
Novikov, D
Novikov, I
Oxborrow, CA
Paci, F
Pagano, L
Pajot, F
Paoletti, D
Pasian, F
Patanchon, G
Peiris, HV
Perdereau, O
Perotto, L
Perrotta, F
Pettorino, V
Piacentini, F
Piat, M
Pierpaoli, E
Pietrobon, D
Plaszczynski, S
Pogosyan, D
Pointecouteau, E
Polenta, G
Popa, L
Pratt, GW
Prezeau, G
Prunet, S
Puget, JL
Rachen, JP
Rebolo, R
Reinecke, M
Remazeilles, M
Renault, C
Renzi, A
Ristorcelli, I
Rocha, G
Rosset, C
Rossetti, M
Roudier, G
Rowan-Robinson, M
Rubino-Martin, JA
Rusholme, B
Sandri, M
Santos, D
Savelainen, M
Savini, G
Scott, D
Seiffert, MD
Shellard, EPS
Spencer, LD
Stolyarov, V
Stompor, R
Sudiwala, R
Sutton, D
Suur-Uski, AS
Sygnet, JF
Tauber, JA
Terenzi, L
Toffolatti, L
Tomasi, M
Tristram, M
Tucci, M
Tuovinen, J
Valenziano, L
Valiviita, J
Van Tent, F
Vielva, P
Villa, F
Wade, LA
Wandelt, BD
Wehus, IK
Yvon, D
Zacchei, A
Zonca, A
AF Ade, P. A. R.
Aghanim, N.
Arnaud, M.
Ashdown, M.
Aumont, J.
Baccigalupi, C.
Banday, A. J.
Barreiro, R. B.
Bartolo, N.
Basak, S.
Battaner, E.
Benabed, K.
Benoit, A.
Benoit-Levy, A.
Bernard, J-P.
Bersanelli, M.
Bielewicz, P.
Bock, J. J.
Bonaldi, A.
Bonavera, L.
Bond, J. R.
Borrill, J.
Bouchet, F. R.
Bucher, M.
Burigana, C.
Butler, R. C.
Calabrese, E.
Cardoso, J. -F.
Catalano, A.
Challinor, A.
Chamballu, A.
Chiang, H. C.
Christensen, P. R.
Church, S.
Clements, D. L.
Colombi, S.
Colombo, L. P. L.
Combet, C.
Couchot, F.
Coulais, A.
Crill, B. P.
Curto, A.
Cuttaia, F.
Danese, L.
Davies, R. D.
Davis, R. J.
de Bernardis, P.
de Rosa, A.
de Zotti, G.
Delabrouille, J.
Desert, F. -X.
Diego, J. M.
Dole, H.
Donzelli, S.
Dore, O.
Douspis, M.
Ducout, A.
Dupac, X.
Efstathiou, G.
Elsner, F.
Ensslin, T. A.
Eriksen, H. K.
Feeney, S.
Fergusson, J.
Finelli, F.
Forni, O.
Frailis, M.
Fraisse, A. A.
Franceschi, E.
Frejse, A.
Galeotta, S.
Galli, S.
Ganga, K.
Giard, M.
Giraud-Heraud, Y.
Gjerlow, E.
Gonzalez-Nuevo, J.
Gorski, K. M.
Gratton, S.
Gregorio, A.
Gruppuso, A.
Gudmundsson, J. E.
Hansen, F. K.
Hanson, D.
Harrison, D. L.
Henrot-Versille, S.
Hernandez-Monteagudo, C.
Herranz, D.
Hildebrandt, S. R.
Hivon, E.
Hobson, M.
Holmes, W. A.
Hornstrup, A.
Hovest, W.
Huffenberger, K. M.
Hurier, G.
Jaffe, A. H.
Jaffe, T. R.
Jones, W. C.
Juvela, M.
Keihanen, E.
Keskitalo, R.
Kisner, T. S.
Knoche, J.
Kunz, M.
Kurki-Suonio, H.
Lagache, G.
Lahteenmaki, A.
Lamarre, J. -M.
Lasenby, A.
Lattanzi, M.
Lawrence, C. R.
Leonardi, R.
Lesgourgues, J.
Levrier, F.
Liguori, M.
Lilje, P. B.
Linden-Vornle, M.
Lopez-Caniego, M.
Lubin, P. M.
Macias-Perez, J. F.
Maggio, G.
Maino, D.
Mandolesi, N.
Mangilli, A.
Maris, M.
Martin, P. G.
Martinez-Gonzalez, E.
Masi, S.
Matarrese, S.
McEwen, J. D.
McGehee, P.
Meinhold, P. R.
Melchiorri, A.
Mendes, L.
Mennella, A.
Migliaccio, M.
Mitra, S.
Miville-Deschenes, M. -A.
Moneti, A.
Montier, L.
Morgante, G.
Mortlock, D.
Moss, A.
Munshi, D.
Murphy, J. A.
Naselsky, P.
Nati, F.
Natoli, P.
Netterfield, C. B.
Norgaard-Nielsen, H. U.
Noviello, F.
Novikov, D.
Novikov, I.
Oxborrow, C. A.
Paci, F.
Pagano, L.
Pajot, F.
Paoletti, D.
Pasian, F.
Patanchon, G.
Peiris, H. V.
Perdereau, O.
Perotto, L.
Perrotta, F.
Pettorino, V.
Piacentini, F.
Piat, M.
Pierpaoli, E.
Pietrobon, D.
Plaszczynski, S.
Pogosyan, D.
Pointecouteau, E.
Polenta, G.
Popa, L.
Pratt, G. W.
Prezeau, G.
Prunet, S.
Puget, J. -L.
Rachen, J. P.
Rebolo, R.
Reinecke, M.
Remazeilles, M.
Renault, C.
Renzi, A.
Ristorcelli, I.
Rocha, G.
Rosset, C.
Rossetti, M.
Roudier, G.
Rowan-Robinson, M.
Rubino-Martin, J. A.
Rusholme, B.
Sandri, M.
Santos, D.
Savelainen, M.
Savini, G.
Scott, D.
Seiffert, M. D.
Shellard, E. P. S.
Spencer, L. D.
Stolyarov, V.
Stompor, R.
Sudiwala, R.
Sutton, D.
Suur-Uski, A. -S.
Sygnet, J. -F.
Tauber, J. A.
Terenzi, L.
Toffolatti, L.
Tomasi, M.
Tristram, M.
Tucci, M.
Tuovinen, J.
Valenziano, L.
Valiviita, J.
Van Tent, F.
Vielva, P.
Villa, F.
Wade, L. A.
Wandelt, B. D.
Wehus, I. K.
Yvon, D.
Zacchei, A.
Zonca, A.
CA Planck Collaboration
TI Planck 2015 results XVIII. Background geometry and topology of the
Universe
SO ASTRONOMY & ASTROPHYSICS
LA English
DT Article
DE cosmic background radiation; cosmology: observations; cosmological
parameters; gravitation; methods: data analysis; methods:statistical
ID DODECAHEDRAL SPACE TOPOLOGY; BIANCHI-VIIH MODELS; WMAP DATA; SKY MAPS;
COBE-DMR; COSMIC CRYSTALLOGRAPHY; COSMOLOGICAL MODELS; TOROIDAL
UNIVERSE; CMB ANISOTROPY; MICROWAVE
AB Maps of cosmic microwave background (CMB) temperature and polarization from the 2015 release of Planck data provide the highest quality full-sky view of the surface of last scattering available to date. This enables us to detect possible departures from a globally isotropic cosmology. We present the first searches using CMB polarization for correlations induced by a possible non-trivial topology with a fundamental domain that intersects, or nearly intersects, the last-scattering surface (at comoving distance chi(rec)), both via a direct scan for matched circular patterns at the intersections and by an optimal likelihood calculation for specific topologies. We specialize to flat spaces with cubic toroidal (T3) and slab (T1) topologies, finding that explicit searches for the latter are sensitive to other topologies with antipodal symmetry. These searches yield no detection of a compact topology with a scale below the diameter of the last-scattering surface. The limits on the radius R-i of the largest sphere inscribed in the fundamental domain (at log-likelihood ratio Delta ln L > -5 relative to a simply-connected flat Planck best-fit model) are: R-i > 0.97 chi(rec) for the T3 cubic torus; and R-i > 0.56 chi(rec) for the T1 slab. The limit for the T3 cubic torus from the matched-circles search is numerically equivalent, R-i > 0.97 chi(rec) at 99% confidence level from polarization data alone. We also perform a Bayesian search for an anisotropic global Bianchi VIIh geometry. In the non-physical setting, where the Bianchi cosmology is decoupled from the standard cosmology, Planck temperature data favour the inclusion of a Bianchi component with a Bayes factor of at least 2.3 units of log-evidence. However, the cosmological parameters that generate this pattern are in strong disagreement with those found from CMB anisotropy data alone. Fitting the induced polarization pattern for this model to the Planck data requires an amplitude of -0.10 +/- 0.04 compared to the value of + 1 if the model were to be correct. In the physically motivated setting, where the Bianchi parameters are coupled and fitted simultaneously with the standard cosmological parameters, we find no evidence for a Bianchi VIIh cosmology and constrain the vorticity of such models to (omega/H)(0) < 7.6 x 10(-10) (95% CL).
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RP Jaffe, AH (reprint author), Imperial Coll London, Astrophys Grp, Blackett Lab, Prince Consort Rd, London SW7 2AZ, England.
EM a.jaffe@imperial.ac.uk
RI Lahteenmaki, Anne/L-5987-2013; Barreiro, Rita Belen/N-5442-2014;
bonavera, laura/E-9368-2017; Gonzalez-Nuevo, Joaquin/I-3562-2014;
Herranz, Diego/K-9143-2014; Colombo, Loris/J-2415-2016;
OI Zacchei, Andrea/0000-0003-0396-1192; Toffolatti,
Luigi/0000-0003-2645-7386; Lilje, Per/0000-0003-4324-7794; Paoletti,
Daniela/0000-0003-4761-6147; Nati, Federico/0000-0002-8307-5088; Savini,
Giorgio/0000-0003-4449-9416; Pierpaoli, Elena/0000-0002-7957-8993;
Juvela, Mika/0000-0002-5809-4834; Valiviita, Jussi/0000-0001-6225-3693;
Kurki-Suonio, Hannu/0000-0002-4618-3063; Barreiro, Rita
Belen/0000-0002-6139-4272; bonavera, laura/0000-0001-8039-3876;
Gonzalez-Nuevo, Joaquin/0000-0003-1354-6822; Herranz,
Diego/0000-0003-4540-1417; Colombo, Loris/0000-0003-4572-7732; Hivon,
Eric/0000-0003-1880-2733; TERENZI, LUCA/0000-0001-9915-6379; Stolyarov,
Vladislav/0000-0001-8151-828X
FU ESA; CNES (France); CNRS/INSU-IN2P3-INP (France); ASI (Italy); CNR
(Italy); INAF (Italy); NASA (USA); DoE (USA); STFC (UK); UKSA (UK); CSIC
(Spain); MINECO (Spain); JA (Spain); RES (Spain); Tekes (Finland); AoF
(Finland); CSC (Finland); DLR (Germany); MPG (Germany); CSA (Canada);
DTU Space (Denmark); SER/SSO (Switzerland); RCN (Norway); SFI (Ireland);
FCT/MCTES (Portugal); ERC (EU); PRACE (EU); Canada Foundation for
Innovation under Compute Canada; Government of Ontario; Ontario Research
Fund Research Excellence; University of Toronto
FX The Planck Collaboration acknowledges the support of: ESA; CNES and
CNRS/INSU-IN2P3-INP (France); ASI, CNR, and INAF (Italy); NASA and DoE
(USA); STFC and UKSA (UK); CSIC, MINECO, JA, and RES (Spain); Tekes,
AoF, and CSC (Finland); DLR and MPG (Germany); CSA (Canada); DTU Space
(Denmark); SER/SSO (Switzerland); RCN (Norway); SFI (Ireland); FCT/MCTES
(Portugal); ERC and PRACE (EU). A description of the Planck
Collaboration and a list of its members, indicating which technical or
scientific activities they have been involved in, can be found at
http://www.cosmos.esa.int/web/planck/planck-collaboration. The authors
thank Andrew Pontzen for computing Bianchi VIIh polarization templates
for the best-fit models resulting from the analysis of temperature data.
We acknowledge the UCL Legion High Performance Computing Facility
(Legion@UCL) and associated support services in the completion of this
work. Parts of the computations were performed on the Andromeda and
Perseus clusters of the University of Geneva, as well as the Carver IBM
iDataPlex, the Hopper Cray XE6, and the Edison Cray XC30 at NERSC, and
on the GPC supercomputer at the SciNet HPC Consortium. SciNet is funded
by: the Canada Foundation for Innovation under the auspices of Compute
Canada; the Government of Ontario; Ontario Research Fund Research
Excellence; and the University of Toronto.
NR 107
TC 0
Z9 0
U1 1
U2 1
PU EDP SCIENCES S A
PI LES ULIS CEDEX A
PA 17, AVE DU HOGGAR, PA COURTABOEUF, BP 112, F-91944 LES ULIS CEDEX A,
FRANCE
SN 1432-0746
J9 ASTRON ASTROPHYS
JI Astron. Astrophys.
PD OCT
PY 2016
VL 594
AR A18
DI 10.1051/0004-6361/201525829
PG 21
WC Astronomy & Astrophysics
SC Astronomy & Astrophysics
GA DZ4MG
UT WOS:000385832200012
ER
PT J
AU Ade, PAR
Aghanim, N
Arnaud, M
Arroja, F
Ashdown, M
Aumont, J
Baccigalupi, C
Ballardini, M
Banday, AJ
Barreiro, RB
Bartolo, N
Battaner, E
Benabed, K
Benoit, A
Benoit-Levy, A
Bernard, JP
Bersanelli, M
Bielewicz, P
Bock, JJ
Bonaldi, A
Bonavera, L
Bond, JR
Borrill, J
Bouchet, FR
Bucher, M
Burigana, C
Butler, RC
Calabrese, E
Cardoso, JF
Catalano, A
Chamballu, A
Chiang, HC
Chluba, J
Christensen, PR
Church, S
Clements, DL
Colombi, S
Colombo, LPL
Combet, C
Couchot, F
Coulais, A
Crill, BP
Curto, A
Cuttaia, F
Danese, L
Davies, RD
Davis, RJ
de Bernardis, P
de Rosa, A
de Zotti, G
Delabrouille, J
Desert, FX
Diego, JM
Dolag, K
Dole, H
Donzelli, S
Dore, A
Douspis, M
Ducout, A
Dupac, X
Efstathiou, G
Elsner, F
Ensslin, TA
Eriksen, HK
Fergusson, J
Finelli, F
Florido, E
Forni, O
Frailis, M
Fraisse, AA
Franceschi, E
Frejsel, A
Galeotta, S
Galli, S
Ganga, K
Giard, M
Giraud-Heraud, Y
Gjerlow, E
Gonzalez-Nuevo, J
Gorski, KM
Gratton, S
Gregorio, A
Gruppuso, A
Gudmundsson, JE
Hansen, FK
Hanson, D
Harrison, DL
Helou, G
Henrot-Versille, S
Hernandez-Monteagudo, C
Herranz, D
Hildebrandt, SR
Hivon, E
Hobson, M
Holmes, WA
Hornstrup, A
Hovest, W
Huffenberger, KM
Hurier, G
Jaffe, AH
Jaffe, TR
Jones, WC
Juvela, M
Keihanen, E
Keskitalo, R
Kim, J
Kisner, TS
Knoche, J
Kunz, M
Kurki-Suonio, H
Lagache, G
Lahteenmaki, A
Lamarre, JM
Lasenby, A
Lattanzi, M
Lawrence, CR
Leahy, JP
Leonardi, R
Lesgourgues, J
Levrier, F
Liguori, M
Lilje, PB
Linden-Vornle, M
Lopez-Caniego, M
Lubin, PM
Macias-Perez, JF
Maggio, G
Maino, D
Mandolesi, N
Mangilli, A
Maris, M
Martin, PG
Martinez-Gonzalez, E
Masi, S
Matarrese, S
McGehee, P
Meinhold, PR
Melchiorri, A
Mendes, L
Mennella, A
Migliaccio, M
Mitra, S
Miville-Deschenes, MA
Molinari, D
Moneti, A
Montier, L
Morgante, G
Mortlock, D
Moss, A
Munshi, D
Murphy, JA
Naselsky, P
Nati, F
Natoli, P
Netterfield, CB
Norgaard-Nielsen, HU
Noviello, F
Novikov, D
Novikov, I
Oppermann, N
Oxborrow, CA
Paci, F
Pagano, L
Pajot, F
Paoletti, D
Pasian, F
Patanchon, G
Perdereau, O
Perotto, L
Perrotta, F
Pettorino, V
Piacentini, F
Piat, M
Pierpaoli, E
Pietrobon, D
Plaszczynski, S
Pointecouteau, E
Polenta, G
Popa, L
Pratt, GW
Prezeau, G
Prunet, S
Puget, JL
Rachen, JP
Rebolo, R
Reinecke, M
Remazeilles, M
Renault, C
Renzi, A
Ristorcelli, I
Rocha, G
Rosset, C
Rossetti, M
Roudier, G
Rubino-Martin, JA
Ruiz-Granados, B
Rusholme, B
Sandri, M
Santos, D
Savelainen, M
Savini, G
Scott, D
Seiffert, MD
Shellard, EPS
Shiraishi, M
Spencer, LD
Stolyarov, V
Stompor, R
Sudiwala, R
Sunyaev, R
Sutton, D
Suur-Uski, AS
Sygnet, JF
Tauber, JA
Terenzi, L
Toffolatti, L
Tomasi, M
Tristram, M
Tucci, M
Tuovinen, J
Umana, G
Valenziano, L
Valiviita, J
Van Tent, B
Vielva, P
Villa, F
Wade, LA
Wandelt, BD
Wehus, IK
Yvon, D
Zacchei, A
Zonca, A
AF Ade, P. A. R.
Aghanim, N.
Arnaud, M.
Arroja, F.
Ashdown, M.
Aumont, J.
Baccigalupi, C.
Ballardini, M.
Banday, A. J.
Barreiro, R. B.
Bartolo, N.
Battaner, E.
Benabed, K.
Benoit, A.
Benoit-Levy, A.
Bernard, J. -P.
Bersanelli, M.
Bielewicz, P.
Bock, J. J.
Bonaldi, A.
Bonavera, L.
Bond, J. R.
Borrill, J.
Bouchet, F. R.
Bucher, M.
Burigana, C.
Butler, R. C.
Calabrese, E.
Cardoso, J. -F.
Catalano, A.
Chamballu, A.
Chiang, H. C.
Chluba, J.
Christensen, P. R.
Church, S.
Clements, D. L.
Colombi, S.
Colombo, L. P. L.
Combet, C.
Couchot, F.
Coulais, A.
Crill, B. P.
Curto, A.
Cuttaia, F.
Danese, L.
Davies, R. D.
Davis, R. J.
de Bernardis, P.
de Rosa, A.
de Zotti, G.
Delabrouille, J.
Desert, F. -X.
Diego, J. M.
Dolag, K.
Dole, H.
Donzelli, S.
Dore, A.
Douspis, M.
Ducout, A.
Dupac, X.
Efstathiou, G.
Elsner, F.
Ensslin, T. A.
Eriksen, H. K.
Fergusson, J.
Finelli, F.
Florido, E.
Forni, O.
Frailis, M.
Fraisse, A. A.
Franceschi, E.
Frejsel, A.
Galeotta, S.
Galli, S.
Ganga, K.
Giard, M.
Giraud-Heraud, Y.
Gjerlow, E.
Gonzalez-Nuevo, J.
Gorski, K. M.
Gratton, S.
Gregorio, A.
Gruppuso, A.
Gudmundsson, J. E.
Hansen, F. K.
Hanson, D.
Harrison, D. L.
Helou, G.
Henrot-Versille, S.
Hernandez-Monteagudo, C.
Herranz, D.
Hildebrandt, S. R.
Hivon, E.
Hobson, M.
Holmes, W. A.
Hornstrup, A.
Hovest, W.
Huffenberger, K. M.
Hurier, G.
Jaffe, A. H.
Jaffe, T. R.
Jones, W. C.
Juvela, M.
Keihanen, E.
Keskitalo, R.
Kim, J.
Kisner, T. S.
Knoche, J.
Kunz, M.
Kurki-Suonio, H.
Lagache, G.
Lahteenmaki, A.
Lamarre, J. -M.
Lasenby, A.
Lattanzi, M.
Lawrence, C. R.
Leahy, J. P.
Leonardi, R.
Lesgourgues, J.
Levrier, F.
Liguori, M.
Lilje, P. B.
Linden-Vornle, M.
Lopez-Caniego, M.
Lubin, P. M.
Macias-Perez, J. F.
Maggio, G.
Maino, D.
Mandolesi, N.
Mangilli, A.
Maris, M.
Martin, P. G.
Martinez-Gonzalez, E.
Masi, S.
Matarrese, S.
McGehee, P.
Meinhold, P. R.
Melchiorri, A.
Mendes, L.
Mennella, A.
Migliaccio, M.
Mitra, S.
Miville-Deschenes, M. -A.
Molinari, D.
Moneti, A.
Montier, L.
Morgante, G.
Mortlock, D.
Moss, A.
Munshi, D.
Murphy, J. A.
Naselsky, P.
Nati, F.
Natoli, P.
Netterfield, C. B.
Norgaard-Nielsen, H. U.
Noviello, F.
Novikov, D.
Novikov, I.
Oppermann, N.
Oxborrow, C. A.
Paci, F.
Pagano, L.
Pajot, F.
Paoletti, D.
Pasian, F.
Patanchon, G.
Perdereau, O.
Perotto, L.
Perrotta, F.
Pettorino, V.
Piacentini, F.
Piat, M.
Pierpaoli, E.
Pietrobon, D.
Plaszczynski, S.
Pointecouteau, E.
Polenta, G.
Popa, L.
Pratt, G. W.
Prezeau, G.
Prunet, S.
Puget, J. -L.
Rachen, J. P.
Rebolo, R.
Reinecke, M.
Remazeilles, M.
Renault, C.
Renzi, A.
Ristorcelli, I.
Rocha, G.
Rosset, C.
Rossetti, M.
Roudier, G.
Rubino-Martin, J. A.
Ruiz-Granados, B.
Rusholme, B.
Sandri, M.
Santos, D.
Savelainen, M.
Savini, G.
Scott, D.
Seiffert, M. D.
Shellard, E. P. S.
Shiraishi, M.
Spencer, L. D.
Stolyarov, V.
Stompor, R.
Sudiwala, R.
Sunyaev, R.
Sutton, D.
Suur-Uski, A. -S.
Sygnet, J. -F.
Tauber, J. A.
Terenzi, L.
Toffolatti, L.
Tomasi, M.
Tristram, M.
Tucci, M.
Tuovinen, J.
Umana, G.
Valenziano, L.
Valiviita, J.
Van Tent, B.
Vielva, P.
Villa, F.
Wade, L. A.
Wandelt, B. D.
Wehus, I. K.
Yvon, D.
Zacchei, A.
Zonca, A.
CA Planck Collaboration
TI Planck 2015 results XIX. Constraints on primordial magnetic fields
SO ASTRONOMY & ASTROPHYSICS
LA English
DT Article
DE magnetic fields; cosmic background radiation; early Universe
ID MICROWAVE BACKGROUND ANISOTROPIES; CMB SPECTRAL DISTORTIONS;
FARADAY-ROTATION; EARLY UNIVERSE; TEV BLAZARS; DENSITY PERTURBATIONS;
CYCLOTRON EMISSION; RADIO-EMISSION; 1ES 0229+200; POLARIZATION
AB We compute and investigate four types of imprint of a stochastic background of primordial magnetic fields (PMFs) on the cosmic microwave background (CMB) anisotropies: the impact of PMFs on the CMB temperature and polarization spectra, which is related to their contribution to cosmological perturbations; the effect on CMB polarization induced by Faraday rotation; the impact of PMFs on the ionization history; magnetically-induced non-Gaussianities and related non-zero bispectra; and the magnetically-induced breaking of statistical isotropy. We present constraints on the amplitude of PMFs that are derived from different Planck data products, depending on the specific effect that is being analysed. Overall, Planck data constrain the amplitude of PMFs to less than a few nanoGauss, with different bounds that depend on the considered model. In particular, individual limits coming from the analysis of the CMB angular power spectra, using the Planck likelihood, are B-1 (Mpc) < 4.4 nG (where B1 Mpc is the comoving field amplitude at a scale of 1 Mpc) at 95% confidence level, assuming zero helicity. By considering the Planck likelihood, based only on parity-even angular power spectra, we obtain B-1 (Mpc) < 5.6 nG for a maximally helical field. For nearly scale-invariant PMFs we obtain B-1 (Mpc) < 2.0 nG and B-1 (Mpc) < 0.9 nG if the impact of PMFs on the ionization history of the Universe is included in the analysis. From the analysis of magnetically-induced non-Gaussianity, we obtain three different values, corresponding to three applied methods, all below 5 nG. The constraint from the magnetically-induced passive-tensor bispectrum is B-1 (Mpc) < 2.8 nG. A search for preferred directions in the magnetically-induced passive bispectrum yields B-1 (Mpc) < 4.5 nG, whereas the compensated-scalar bispectrum gives B-1 (Mpc) < 3 nG. The analysis of the Faraday rotation of CMB polarization by PMFs uses the Planck power spectra in EE and BB at 70 GHz and gives B-1 (Mpc) < 1380 nG. In our final analysis, we consider the harmonic-space correlations produced by Alfven waves, finding no significant evidence for the presence of these waves. Together, these results comprise a comprehensive set of constraints on possible PMFs with Planck data.
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[Lahteenmaki, A.] Aalto Univ, Metsahovi Radio Observ, POB 13000, Aalto 00076, Finland.
[Lahteenmaki, A.] Aalto Univ, Dept Radio Sci & Engn, POB 13000, Aalto 00076, Finland.
[Kunz, M.] African Inst Math Sci, 6-8 Melrose Rd, ZA-7945 Cape Town, South Africa.
[Natoli, P.; Polenta, G.] Agenzia Spaziale Italiana, Sci Data Ctr, Via Politecn Snc, I-00133 Rome, Italy.
[Lagache, G.] Aix Marseille Univ, CNRS, LAM, UMR 7326, F-13388 Marseille, France.
[Ashdown, M.; Curto, A.; Hobson, M.; Lasenby, A.; Stolyarov, V.] Univ Cambridge, Astrophys Grp, Cavendish Lab, JJ Thomson Ave, Cambridge CB3 0HE, England.
[Chiang, H. C.] Univ KwaZulu Natal, Astrophys & Cosmol Res Unit, Sch Math Stat & Comp Sci, Westville Campus,Private Bag X54001, ZA-4000 Durban, South Africa.
[Leonardi, R.] Ed Parque Cidade Corp, CGEE, Lote C, Torre C, SCS Qd 9,4o andar, BR-70308200 Brasilia, DF, Brazil.
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[Tuovinen, J.] Trinity Coll Dublin, CRANN, Dublin 2, Ireland.
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[Hernandez-Monteagudo, C.] CEFCA, Plaza San Juan,1,Planta 2, Teruel 44001, Spain.
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[Huffenberger, K. M.] Florida State Univ, Dept Phys, Keen Phys Bldg,77 Chieftan Way, Tallahassee, FL 32306 USA.
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[Chiang, H. C.; Fraisse, A. A.; Gudmundsson, J. E.; Jones, W. C.; Nati, F.] Princeton Univ, Dept Phys, Princeton, NJ 08544 USA.
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[Bartolo, N.; Liguori, M.; Matarrese, S.; Shiraishi, M.] Univ Padua, Dipartimento Fis & Astron G Galilei, Via Marzolo 8, I-35131 Padua, Italy.
[Ballardini, M.] Univ Bologna, Dipartimento Fis & Astron, ALMA MATER STUDIORUM, Viale Berti Pichat 6-2, I-40127 Bologna, Italy.
[Burigana, C.; Lattanzi, M.; Mandolesi, N.; Natoli, P.] Univ Ferrara, Dipartimento Fis & Sci Terra, Via Saragat 1, I-44122 Ferrara, Italy.
[de Bernardis, P.; Masi, S.; Melchiorri, A.; Pagano, L.; Piacentini, F.] Univ Roma La Sapienza, Dipartimento Fis, Ple A Moro 2, I-00185 Rome, Italy.
[Bersanelli, M.; Maino, D.; Mennella, A.; Rossetti, M.; Tomasi, M.] Univ Milan, Dipartimento Fis, Via Celoria 16, I-20133 Milan, Italy.
[Gregorio, A.] Univ Trieste, Dipartimento Fis, Via A Valerio 2, I-34127 Trieste, Italy.
[Renzi, A.] Univ Roma Tor Vergata, Dipartimento Matemat, Via Ric Sci 1, I-00133 Rome, Italy.
[Christensen, P. R.] Niels Bohr Inst, Discovery Ctr, Blegdamsvej 17, DK-2100 Copenhagen, Denmark.
[Naselsky, P.] Univ Copenhagen, Niels Bohr Inst, Discovery Ctr, Blegdamsvej 17, DK-2100 Copenhagen, Denmark.
[Dupac, X.; Lopez-Caniego, M.; Mendes, L.] European Space Agcy, ESAC, Planck Sci Off, Camino Bajo Castillo S-N, Madrid 28692, Spain.
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[Pettorino, V.] HGSFP, Philosophenweg 16, D-69120 Heidelberg, Germany.
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[Umana, G.] INAF Osservatorio Astrofis Catania, Via S Sofia 78, I-95123 Catania, Italy.
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[Ballardini, M.; Burigana, C.; Finelli, F.; Paoletti, D.] INFN, Sez Bologna, Via Irnerio 46, I-40126 Bologna, Italy.
[Melchiorri, A.; Pagano, L.] Univ Roma Sapienza, INFN, Sez Roma 1, Piazzale Aldo Moro 2, I-00185 Rome, Italy.
[Renzi, A.] Univ Roma Tor Vergata, INFN, Sez Roma 2, Via Ric Sci 1, I-00185 Rome, Italy.
[Gregorio, A.] INFN Natl Inst Nucl Phys, Via Valerio 2, I-34127 Trieste, Italy.
[Desert, F. -X.] Univ Grenoble Alpes, IPAG, CNRS, F-38000 Grenoble, France.
[Mitra, S.] IUCAA, Post Bag 4,Pune Univ Campus, Pune 411007, Maharashtra, India.
[Clements, D. L.; Ducout, A.; Jaffe, A. H.; Mortlock, D.] Imperial Coll London, Blackett Lab, Astrophys Grp, Prince Consort Rd, London SW7 2AZ, England.
[McGehee, P.; Rusholme, B.] CALTECH, Infrared Proc & Anal Ctr, Pasadena, CA 91125 USA.
[Benoit, A.] Univ Joseph Fourier Grenoble I, CNRS, Inst Neel, 25 Rue Martyrs, Grenoble, France.
[Dole, H.] Inst Univ France, 103 Bd St Michel, F-75005 Paris, France.
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[Benabed, K.; Benoit-Levy, A.; Bouchet, F. R.; Cardoso, J. -F.; Colombi, S.; Ducout, A.; Elsner, F.; Hivon, E.; Moneti, A.; Prunet, S.; Sygnet, J. -F.; Wandelt, B. D.] CNRS, Inst Astrophys Paris, UMR 7095, 98 Bis Blvd Arago, F-75014 Paris, France.
[Lesgourgues, J.] Rhein Westfal TH Aachen, Inst Theoret Teilchenphys & Kosmol, D-52056 Aachen, Germany.
[Popa, L.] Inst Space Sci, Bucharest 077125, Romania.
[Efstathiou, G.; Gratton, S.; Harrison, D. L.; Migliaccio, M.; Sutton, D.] Univ Cambridge, Inst Astron, Madingley Rd, Cambridge CB3 0HA, England.
[Eriksen, H. K.; Gjerlow, E.; Hansen, F. K.; Lilje, P. B.; Wehus, I. K.] Univ Oslo, Inst Theoret Astrophys, N-0371 Oslo, Norway.
[Rebolo, R.; Rubino-Martin, J. A.] Inst Astrofis Canarias, C Via Lactea S-N, Tenerife 38205, Spain.
[Barreiro, R. B.; Bonavera, L.; Curto, A.; Diego, J. M.; Gonzalez-Nuevo, J.; Herranz, D.; Lopez-Caniego, M.; Martinez-Gonzalez, E.; Molinari, D.; Toffolatti, L.; Vielva, P.] Univ Cantabria, CSIC, Inst Fis Cantabria, Avda Castros S-N, E-39005 Santander, Spain.
[Arroja, F.; Bartolo, N.; Liguori, M.; Matarrese, S.; Shiraishi, M.] Ist Nazl Fis Nucl, Sez Padova, Via Marzolo 8, I-35131 Padua, Italy.
[Bock, J. J.; Colombo, L. P. L.; Crill, B. P.; Dore, A.; Gorski, K. M.; Hanson, D.; Hildebrandt, S. R.; Holmes, W. A.; Lawrence, C. R.; Mitra, S.; Pietrobon, D.; Prezeau, G.; Rocha, G.; Roudier, G.; Seiffert, M. D.; Wade, L. A.; Wehus, I. K.] CALTECH, Jet Prop Lab, 4800 Oak Grove Dr, Pasadena, CA USA.
[Bonaldi, A.; Davies, R. D.; Davis, R. J.; Leahy, J. P.; Noviello, F.; Remazeilles, M.] Univ Manchester, Jodrell Bank Ctr Astrophys, Sch Phys & Astron, Alan Turing Bldg,Oxford Rd, Manchester M13 9PL, Lancs, England.
[Galli, S.] Univ Chicago, Kavli Inst Cosmol Phys, Chicago, IL 60637 USA.
[Ashdown, M.; Chluba, J.; Curto, A.; Gratton, S.; Harrison, D. L.; Lasenby, A.; Migliaccio, M.; Sutton, D.] Kavli Inst Cosmol Cambridge, Madingley Rd, Cambridge CB3 0HA, England.
[Stolyarov, V.] Kazan Fed Univ, 18 Kremlyovskaya St, Kazan 420008, Russia.
[Couchot, F.; Henrot-Versille, S.; Mangilli, A.; Perdereau, O.; Plaszczynski, S.; Tristram, M.] Univ Paris 11, LAL, CNRS IN2P3, F-91898 Orsay, France.
[Catalano, A.; Coulais, A.; Lamarre, J. -M.; Levrier, F.; Roudier, G.] CNRS, LERMA, Observ Paris, 61 Ave Observ, F-75014 Paris, France.
[Arnaud, M.; Chamballu, A.; Pratt, G. W.] Univ Paris Diderot, CEA Saclay, CNRS, Lab AIM,IRFU Serv Astrophys,CEA DSM, Bat 709, F-91191 Gif Sur Yvette, France.
[Cardoso, J. -F.] CNRS, Lab Traitement & Commun Informat, UMR 5141, 46 Rue Barrault, F-75634 Paris 13, France.
[Cardoso, J. -F.] Telecom ParisTech, 46 Rue Barrault, F-75634 Paris 13, France.
[Catalano, A.; Combet, C.; Macias-Perez, J. F.; Perotto, L.; Renault, C.; Santos, D.] Univ Grenoble Alpes, CNRS IN2P3, Lab Phys Subatom & Cosmol, 53 Rue Martyrs, F-38026 Grenoble, France.
[Van Tent, B.] Univ Paris Sud 11, Lab Phys Theor, Batiment 210, F-91405 Orsay, France.
[Van Tent, B.] CNRS, Batiment 210, F-91405 Orsay, France.
[Kisner, T. S.] Lawrence Berkeley Natl Lab, Berkeley, CA 94720 USA.
[Novikov, D.; Novikov, I.] Russian Acad Sci, Lebedev Phys Inst, Ctr Astro Space, 84-32 Profsoyuznaya St, Moscow 117997, Russia.
[Arroja, F.] Natl Taiwan Univ, Leung Ctr Cosmol & Particle Astrophys, Taipei 10617, Taiwan.
[Dolag, K.; Ensslin, T. A.; Hernandez-Monteagudo, C.; Hovest, W.; Kim, J.; Knoche, J.; Rachen, J. P.; Reinecke, M.; Sunyaev, R.] Max Planck Inst Astrophys, Karl Schwarzschild Str 1, D-85741 Garching, Germany.
[Hanson, D.] McGill Univ, McGill Phys, Ernest Rutherford Phys Bldg,3600 Rue Univ, Montreal, PQ H3A 2T8, Canada.
[Murphy, J. A.] Natl Univ Ireland, Dept Expt Phys, Maynooth, Kildare, Ireland.
[Bielewicz, P.] Nicolaus Copernicus Astron Ctr, Bartycka 18, PL-00716 Warsaw, Poland.
[Christensen, P. R.; Frejsel, A.; Novikov, I.] Niels Bohr Inst, Blegdamsvej 17, DK-2100 Copenhagen, Denmark.
[Naselsky, P.] Univ Copenhagen, Niels Bohr Inst, Blegdamsvej 17, DK-2100 Copenhagen, Denmark.
[Gudmundsson, J. E.] Nordita Nord Inst Theoret Phys, Roslagstullsbacken 23, S-10691 Stockholm, Sweden.
[Savini, G.] UCL, Opt Sci Lab, Gower St, London WC1E 6BT, England.
[Baccigalupi, C.; Bielewicz, P.; Danese, L.; de Zotti, G.; Paci, F.; Perrotta, F.] SISSA, Astrophys Sector, Via Bonomea 265, I-34136 Trieste, Italy.
[Terenzi, L.] Univ E Campus, SMARTEST Res Ctr, Via Isimbardi 10, I-22060 Novedrate, CO, Italy.
[Ade, P. A. R.; Munshi, D.; Spencer, L. D.; Sudiwala, R.] Cardiff Univ, Sch Phys & Astron, Queens Bldg, Cardiff CF24 3AA, S Glam, Wales.
[Moss, A.] Univ Nottingham, Sch Phys & Astron, Nottingham NG7 2RD, England.
[Bouchet, F. R.] Sorbonne Univ UPMC, UMR 7095, Inst Astrophys Paris, 98 Bis Blvd Arago, F-75014 Paris, France.
[Sunyaev, R.] Russian Acad Sci, Space Res Inst IKI, Profsoyuznaya Str 84-32, Moscow 117997, Russia.
[Borrill, J.] Univ Calif Berkeley, Space Sci Lab, Berkeley, CA 94720 USA.
[Stolyarov, V.] Russian Acad Sci, Special Astrophys Observ, Karachai Cherkessian Rep 369167, Russia.
[Church, S.] Stanford Univ, Dept Phys, Varian Phys Bldg,382 Via Pueblo Mall, Stanford, CA 94305 USA.
[Calabrese, E.] Univ Oxford, Sub Dept Astrophys, Keble Rd, Oxford OX1 3RH, England.
[Gudmundsson, J. E.] Stockholm Univ, Dept Phys, Oskar Klein Ctr Cosmoparticle Phys, S-10691 Stockholm, Sweden.
[Lesgourgues, J.] CERN, Div Theory, PH TH, CH-1211 Geneva 23, Switzerland.
[Benabed, K.; Benoit-Levy, A.; Colombi, S.; Elsner, F.; Hivon, E.; Prunet, S.; Wandelt, B. D.] UPMC Univ Paris 06, UMR7095, 98 Bis Blvd Arago, F-75014 Paris, France.
[Banday, A. J.; Bernard, J. -P.; Forni, O.; Giard, M.; Jaffe, T. R.; Montier, L.; Pointecouteau, E.; Ristorcelli, I.] Univ Toulouse, UPS OMP, IRAP, F-31028 Toulouse 4, France.
[Dolag, K.] Ludwig Maximilian Univ Munich, Univ Observ, Scheinerstr 1, D-81679 Munich, Germany.
[Battaner, E.; Florido, E.; Ruiz-Granados, B.] Univ Granada, Fac Ciencias, Dept Fis Teor & Cosmos, E-18071 Granada, Spain.
[Battaner, E.] Univ Granada, Inst Carlos Fis Teor & Computac 1, E-18071 Granada, Spain.
[Gorski, K. M.] Univ Warsaw Observ, Aleje Ujazdowskie 4, PL-00478 Warsaw, Poland.
RP Paoletti, D (reprint author), INAF IASF Bologna, Via Gobetti 101, I-40129 Bologna, Italy.; Paoletti, D (reprint author), INFN, Sez Bologna, Via Irnerio 46, I-40126 Bologna, Italy.
EM paoletti@iasfbo.inaf.it
RI Barreiro, Rita Belen/N-5442-2014; bonavera, laura/E-9368-2017;
Gonzalez-Nuevo, Joaquin/I-3562-2014; Herranz, Diego/K-9143-2014;
Colombo, Loris/J-2415-2016; Lahteenmaki, Anne/L-5987-2013
OI Juvela, Mika/0000-0002-5809-4834; Hurier, Guillaume/0000-0002-1215-0706;
Piacentini, Francesco/0000-0002-5444-9327; Molinari,
Diego/0000-0002-7799-3915; Hivon, Eric/0000-0003-1880-2733; Toffolatti,
Luigi/0000-0003-2645-7386; Lilje, Per/0000-0003-4324-7794; Paoletti,
Daniela/0000-0003-4761-6147; Nati, Federico/0000-0002-8307-5088; Savini,
Giorgio/0000-0003-4449-9416; Pierpaoli, Elena/0000-0002-7957-8993;
Barreiro, Rita Belen/0000-0002-6139-4272; bonavera,
laura/0000-0001-8039-3876; Gonzalez-Nuevo, Joaquin/0000-0003-1354-6822;
Herranz, Diego/0000-0003-4540-1417; Colombo, Loris/0000-0003-4572-7732;
Valiviita, Jussi/0000-0001-6225-3693; Kurki-Suonio,
Hannu/0000-0002-4618-3063; Zacchei, Andrea/0000-0003-0396-1192;
Stolyarov, Vladislav/0000-0001-8151-828X; TERENZI,
LUCA/0000-0001-9915-6379;
FU ESA; CNES (France); CNRS/INSU-IN2P3-INP (France); ASI (Italy); CNR
(Italy); INAF (Italy); NASA (USA); DoE (USA); STFC (UK); UKSA (UK); CSIC
(Spain); MINECO (Spain); JA (Spain); RES (Spain); Tekes (Finland); AoF
(Finland); CSC (Finland); DLR (Germany); MPG (Germany); CSA (Canada);
DTU Space (Denmark); SER/SSO (Switzerland); RCN (Norway); SFI (Ireland);
FCT/MCTES (Portugal); ERC (EU); PRACE (EU); Office of Science of the US
Department of Energy [DE-AC02-05CH11231]
FX The Planck Collaboration acknowledges the support of: ESA; CNES and
CNRS/INSU-IN2P3-INP (France); ASI, CNR, and INAF (Italy); NASA and DoE
(USA); STFC and UKSA (UK); CSIC, MINECO, JA, and RES (Spain); Tekes,
AoF, and CSC (Finland); DLR and MPG (Germany); CSA (Canada); DTU Space
(Denmark); SER/SSO (Switzerland); RCN (Norway); SFI (Ireland); FCT/MCTES
(Portugal); ERC and PRACE (EU). A description of the Planck
Collaboration and a list of its members, indicating which technical or
scientific activities they have been involved in, can be found at
http//www.cosmos.esa.int/web/planck/planck-collaboration. This research
used resources of the National Energy Research Scientific Computing
Center, a DOE Office of Science User Facility supported by the Office of
Science of the US Department of Energy under Contract No.
DE-AC02-05CH11231. Some of the results in this paper have been derived
using the HEALPix package.
NR 171
TC 3
Z9 3
U1 2
U2 2
PU EDP SCIENCES S A
PI LES ULIS CEDEX A
PA 17, AVE DU HOGGAR, PA COURTABOEUF, BP 112, F-91944 LES ULIS CEDEX A,
FRANCE
SN 1432-0746
J9 ASTRON ASTROPHYS
JI Astron. Astrophys.
PD OCT
PY 2016
VL 594
AR A19
DI 10.1051/0004-6361/201525821
PG 27
WC Astronomy & Astrophysics
SC Astronomy & Astrophysics
GA DZ4MG
UT WOS:000385832200009
ER
PT J
AU Ade, PAR
Aghanim, N
Arnaud, M
Ashdow, M
Aumont, J
Baccigalupi, C
Banday, AJ
Barreiro, RB
Bartolo, N
Battaner, E
Benabed, K
Benoit, A
Benoit-Levy, A
Bernard, JP
Bersanelli, M
Bielewicz, P
Bonaldi, A
Bonavera, L
Bond, JR
Borrill, J
Bouchet, FR
Boulanger, F
Bucher, M
Burigana, C
Butler, RC
Calabrese, E
Catalano, A
Chamballu, A
Chiang, HC
Christensen, PR
Clements, DL
Colombi, S
Colombo, LPL
Combet, C
Couchot, F
Coulais, A
Crill, BP
Curto, A
Cuttaia, F
Danese, L
Davies, RD
Davis, RJ
de Bernardis, P
de Rosa, A
de Zotti, G
Delabrouille, J
Desert, FX
Dickinson, C
Diego, JM
Dole, H
Donzelli, S
Dore, O
Douspis, M
Ducout, A
Dupac, X
Efstathiou, G
Elsner, F
Ensslin, TA
Eriksen, HK
Falgarone, E
Fergusson, J
Finelli, F
Forni, O
Frailis, M
Fraisse, AA
Franceschi, E
Frejsel, A
Galeotta, S
Galli, S
Ganga, K
Giard, M
Giraud-Heraud, Y
Gjerlow, E
Gonzalez-Nuevo, J
Gorski, KM
Gratton, S
Gregorio, A
Gruppuso, A
Gudmundsson, JE
Hansen, FK
Hanson, D
Harrison, DL
Helou, G
Henrot-Versille, S
Hernandez-Monteagudo, C
Herranz, D
Hildebrandt, SR
Hivon, E
Hobson, M
Holmes, WA
Hornstrup, A
Hovest, W
Huffenberger, KM
Hurier, G
Jaffe, AH
Jaffe, TR
Jones, WC
Juvela, M
Keihanen, E
Keskitalo, R
Kisner, TS
Knoche, J
Kunz, M
Kurki-Suonio, H
Lamarre, JM
Lasenby, A
Lattanzi, M
Lawrence, CR
Leonardi, R
Lesgourgues, J
Levrier, F
Liguori, M
Lilje, PB
Linden-Vornle, M
Lopez-Caniego, M
Lubin, PM
Macias-Perez, JF
Maggio, G
Maino, D
Mandolesi, N
Mangilli, A
Marshall, DJ
Martin, PG
Martinez-Gonzalez, E
Masi, S
Matarrese, S
Mazzotta, P
McGehee, P
Melchiorri, A
Mendes, L
Mennella, A
Migliaccio, M
Mitra, S
Miville-Deschenes, MA
Moneti, A
Montier, L
Morgante, G
Mortlock, D
Moss, A
Munshi, D
Murphy, JA
Naselsky, P
Nati, F
Natoli, P
Netterfield, CB
Norgaard-Nielsen, HU
Noviello, F
Novikov, D
Novikov, I
Oxborrow, CA
Paci, F
Pagano, L
Pajot, F
Paladini, R
Paoletti, D
Pasian, F
Patanchon, G
Pearson, TJ
Pelkonen, VM
Perdereau, O
Perotto, L
Perrotta, F
Pettorino, V
Piacentini, F
Piat, M
Pierpaoli, E
Pietrobon, D
Plaszczynski, S
Pointccoutcau, E
Polcnta, G
Pratt, GW
Prczcau, G
Prunt, S
Pugct, JL
Rachcn, JP
Rcach, WT
Rebolo, R
Reinecke, M
Remazeilles, M
Renault, C
Renzi, A
Ristorcelli, I
Rocha, G
Rosset, C
Rossetti, M
Roudier, G
Rubino-Martin, JA
Rusholme, B
Sandri, M
Santos, D
Savelainen, M
Savini, G
Scott, D
Seiffert, MD
Shellard, EPS
Spencer, LD
Stolyarov, V
Sudiwala, R
Sunyaev, R
Sutton, D
Suur-Uski, AS
Sygnet, JF
Tauber, JA
Tcrcnzi, L
Toffolatti, L
Tomasi, M
Tristram, M
Tucci, M
Tuovincn, J
Umana, G
Valcnziano, L
Valiviita, J
Van Tent, B
Vielva, P
Villa, F
Wade, LA
Wandelt, BD
Wehus, IK
Yvon, D
Zacchei, A
Zonca, A
AF Ade, P. A. R.
Aghanim, N.
Arnaud, M.
Ashdow, M.
Aumont, J.
Baccigalupi, C.
Banday, A. J.
Barreiro, R. B.
Bartolo, N.
Battaner, E.
Benabed, K.
Benoit, A.
Benoit-Levy, A.
Bernard, J. P.
Bersanelli, M.
Bielewicz, P.
Bonaldi, A.
Bonavera, L.
Bond, J. R.
Borrill, J.
Bouchet, F. R.
Boulanger, F.
Bucher, M.
Burigana, C.
Butler, R. C.
Calabrese, E.
Catalano, A.
Chamballu, A.
Chiang, H. C.
Christensen, P. R.
Clements, D. L.
Colombi, S.
Colombo, L. P. L.
Combet, C.
Couchot, F.
Coulais, A.
Crill, B. P.
Curto, A.
Cuttaia, F.
Danese, L.
Davies, R. D.
Davis, R. J.
de Bernardis, P.
de Rosa, A.
de Zotti, G.
Delabrouille, J.
Desert, F. X.
Dickinson, C.
Diego, J. M.
Dole, H.
Donzelli, S.
Dore, O.
Douspis, M.
Ducout, A.
Dupac, X.
Efstathiou, G.
Elsner, F.
Ensslin, T. A.
Eriksen, H. K.
Falgarone, E.
Fergusson, J.
Finelli, F.
Forni, O.
Frailis, M.
Fraisse, A. A.
Franceschi, E.
Frejsel, A.
Galeotta, S.
Galli, S.
Ganga, K.
Giard, M.
Giraud-Heraud, Y.
Gjerlow, E.
Gonzalez-Nuevo, J.
Gorski, K. M.
Gratton, S.
Gregorio, A.
Gruppuso, A.
Gudmundsson, J. E.
Hansen, F. K.
Hanson, D.
Harrison, D. L.
Helou, G.
Henrot-Versille, S.
Hernandez-Monteagudo, C.
Herranz, D.
Hildebrandt, S. R.
Hivon, E.
Hobson, M.
Holmes, W. A.
Hornstrup, A.
Hovest, W.
Huffenberger, K. M.
Hurier, G.
Jaffe, A. H.
Jaffe, T. R.
Jones, W. C.
Juvela, M.
Keihanen, E.
Keskitalo, R.
Kisner, T. S.
Knoche, J.
Kunz, M.
Kurki-Suonio, H.
Lamarre, J. M.
Lasenby, A.
Lattanzi, M.
Lawrence, C. R.
Leonardi, R.
Lesgourgues, J.
Levrier, F.
Liguori, M.
Lilje, P. B.
Linden-Vornle, M.
Lopez-Caniego, M.
Lubin, P. M.
Macias-Perez, J. F.
Maggio, G.
Maino, D.
Mandolesi, N.
Mangilli, A.
Marshall, D. J.
Martin, P. G.
Martinez-Gonzalez, E.
Masi, S.
Matarrese, S.
Mazzotta, P.
McGehee, P.
Melchiorri, A.
Mendes, L.
Mennella, A.
Migliaccio, M.
Mitra, S.
Miville-Deschenes, M. A.
Moneti, A.
Montier, L.
Morgante, G.
Mortlock, D.
Moss, A.
Munshi, D.
Murphy, J. A.
Naselsky, P.
Nati, F.
Natoli, P.
Netterfield, C. B.
Norgaard-Nielsen, H. U.
Noviello, F.
Novikov, D.
Novikov, I.
Oxborrow, C. A.
Paci, F.
Pagano, L.
Pajot, F.
Paladini, R.
Paoletti, D.
Pasian, F.
Patanchon, G.
Pearson, T. J.
Pelkonen, V. M.
Perdereau, O.
Perotto, L.
Perrotta, F.
Pettorino, V.
Piacentini, F.
Piat, M.
Pierpaoli, E.
Pietrobon, D.
Plaszczynski, S.
Pointccoutcau, E.
Polcnta, G.
Pratt, G. W.
Prczcau, G.
Prunct, S.
Pugct, J. L.
Rachcn, J. P.
Rcach, W. T.
Rebolo, R.
Reinecke, M.
Remazeilles, M.
Renault, C.
Renzi, A.
Ristorcelli, I.
Rocha, G.
Rosset, C.
Rossetti, M.
Roudier, G.
Rubino-Martin, J. A.
Rusholme, B.
Sandri, M.
Santos, D.
Savelainen, M.
Savini, G.
Scott, D.
Seiffert, M. D.
Shellard, E. P. S.
Spencer, L. D.
Stolyarov, V.
Sudiwala, R.
Sunyaev, R.
Sutton, D.
Suur-Uski, A. S.
Sygnet, J. F.
Tauber, J. A.
Tcrcnzi, L.
Toffolatti, L.
Tomasi, M.
Tristram, M.
Tucci, M.
Tuovincn, J.
Umana, G.
Valcnziano, L.
Valiviita, J.
Van Tent, B.
Vielva, P.
Villa, F.
Wade, L. A.
Wandelt, B. D.
Wehus, I. K.
Yvon, D.
Zacchei, A.
Zonca, A.
CA Planck Collaboration
TI Planck 2015 results XXVIII. The Planck Catalogue of Galactic cold clumps
SO ASTRONOMY & ASTROPHYSICS
LA English
DT Article
DE ISM: clouds; ISM: structure; local insterstellar matter; stars:
formation
ID INFRARED DARK CLOUDS; SMALL-MAGELLANIC-CLOUD; YOUNG STELLAR OBJECTS;
MOLECULAR CLOUDS; MILKY-WAY; PRESTELLAR CORES; DUST TEMPERATURE;
STAR-FORMATION; INITIAL HIGHLIGHTS; GAS TEMPERATURE
AB We present the Planck Catalogue of Galactic Cold Clumps (PGCC), an all-sky catalogue of Galactic cold clump candidates detected by Planck. This catalogue is the full version of the Early Cold Core (ECC) catalogue, which was made available in 2011 with the Early Release Compact Source Catalogue (ERCSC) and which contained 915 high signal-to-noise sources. It is based on the Planck 48-month mission data that are currently being released to the astronomical community. The PGCC catalogue is an observational catalogue consisting exclusively of Galactic cold sources. The three highest Planck bands (857, 454, and 353 GHz) have been combined with IRAS data at 3 THz to perform a multi-frequency detection of sources colder than their local environment. After rejection of possible extragalactic contaminants, the PGCC catalogue contains 13188 Galactic sources spread across the whole sky, i.e., from the Galactic plane to high latitudes, following the spatial distribution of the main molecular cloud complexes. The median temperature of PGCC sources lies between 13 and 14.5K, depending on the quality of the flux density measurements, with a temperature ranging from 5.8 to 20K after removing the sources with the top 1% highest temperature estimates. Using seven independent methods, reliable distance estimates have been obtained for 5574 sources, which allows us to derive their physical properties such as their mass, physical size, mean density, and luminosity. The PGCC sources are located mainly in the solar neighbourhood, but also up to a distance of 10.5 kpc in the direction of the Galactic centre, and range from low-mass cores to large molecular clouds. Because of this diversity and because the PGCC catalogue contains sources in very different environments, the catalogue is useful for investigating the evolution from molecular clouds to cores. Finally, it also includes 54 additional sources located in the Small and Large Magellanic Clouds.
C1 [Bucher, M.; Delabrouille, J.; Ganga, K.; Giraud-Heraud, Y.; Patanchon, G.; Piat, M.; Remazeilles, M.; Rosset, C.; Roudier, G.] Univ Paris Diderot, Sorbonne Paris Cite, CNRS,IN2P3, APC,AstroParticule & Cosmol,Observ Paris,CEA,Lrfu, F-75205 Paris 13, France.
[Kunz, M.] African Inst Math Sci, 6-8 Melrose Rd, Cape Town, South Africa.
[Natoli, P.; Polcnta, G.] Agenzia Spaziale Italiana Sci, Ctr Data, Via Politecn Snc, I-00133 Rome, Italy.
Aix Marseille Univ, CNRS, LAM, UMR 7326, F-13388 Marseille, France.
[Ashdow, M.; Curto, A.; Hobson, M.; Lasenby, A.; Stolyarov, V.] Univ Cambridge, Astrophys Grp, Cavendish Lab, JJ Thomson Ave, Cambridge CB3 0HE, England.
[Chiang, H. C.] Univ KwaZulu Natal, Sch Math Stat & Comp Sci, Astrophys & Cosmol Res Unit, Westville Campus,Private Bag X54001, ZA-4000 Durban, South Africa.
[Bond, J. R.; Hanson, D.; Martin, P. G.; Miville-Deschenes, M. A.] Univ Toronto, CITA, 60 St George St, Toronto, ON M5S 3H8, Canada.
[Banday, A. J.; Bernard, J. P.; Bielewicz, P.; Forni, O.; Giard, M.; Jaffe, T. R.; Montier, L.; Pointccoutcau, E.; Ristorcelli, I.] IRAP, CNRS, 9 Av Colonel Roche,BP 44346, F-112AP Toulouse 4, France.
[Tuovincn, J.] Trinity Coll Dublin, CRANN, Dublin, Ireland.
[Crill, B. P.; Dore, O.; Helou, G.; Hildebrandt, S. R.; Pearson, T. J.; Prczcau, G.; Rocha, G.; Seiffert, M. D.] CALTECH, Pasadena, CA 91125 USA.
[Fergusson, J.; Shellard, E. P. S.] Univ Cambridge, DAMTP, Ctr Theoret Cosmol, Wilberforce Rd, Cambridge CB3 0WA, England.
[Hernandez-Monteagudo, C.] CEFCA, Plaza San Juan 1,Planta 2, Teruel 44001, Spain.
[Borrill, J.; Keskitalo, R.] Lawrence Berkeley Natl Lab, Computat Cosmol Ctr, Berkeley, CA USA.
[Rebolo, R.] CSIC, Madrid, Spain.
[Chamballu, A.; Yvon, D.] CEA Saclay, DSM, Irfu, SPP, F-91191 Gif Sur Yvette, France.
[Hornstrup, A.; Linden-Vornle, M.; Norgaard-Nielsen, H. U.; Oxborrow, C. A.] Tech Univ Denmark, Natl Space Inst, DTU Space, Elektrovej 327, DK-2800 Lyngby, Denmark.
[Kunz, M.; Tucci, M.] Univ Geneva, Dept Phys Theor, 24 Quai E Ansermet, CH-1211 Geneva 4, Switzerland.
[Toffolatti, L.] Univ Oviedo, Dept Fis, Avda Calvo Sotelo S-N, Oviedo, Spain.
[Netterfield, C. B.] Univ Toronto, Dept Astron & Astrophys, 50 St George St, Toronto, ON, Canada.
[Rachcn, J. P.] Radboud Univ Nijmegen, Dept Astrophys IMAPP, POB 9010, NL-6500 GL Nijmegen, Netherlands.
[Scott, D.] Univ British Columbia, Dept Phys & Astron, 6224 Agr Rd, Vancouver, BC, Canada.
[Benoit-Levy, A.; Elsner, F.] Univ So Calif, Dept Phys & Astron, Dana & David Dornsife Coll Letter Arts & Sci, Los Angeles, CA 90089 USA.
[Benoit-Levy, A.; Elsner, F.] UCL, Dept Phys & Astron, Mortimer St, London WC1E 6BT, England.
[Huffenberger, K. M.] Florida State Univ, Dept Phys, Keen Phys Bldg,77 Chieftan Way, Tallahassee, FL 32306 USA.
[Juvela, M.; Keihanen, E.; Kurki-Suonio, H.; Savelainen, M.; Suur-Uski, A. S.; Valiviita, J.] Univ Helsinki, Dept Phys, Gustaf Hallstromin Katu 2a, SF-00100 Helsinki, Finland.
[Chiang, H. C.; Fraisse, A. A.; Gudmundsson, J. E.; Jones, W. C.; Nati, F.] Princeton Univ, Dept Phys, Princeton, NJ 00185 USA.
[Lubin, P. M.; Zonca, A.] Univ Calif Santa Barbara, Dept Phys, Santa Barbara, CA 93106 USA.
[Wandelt, B. D.] Univ Illinois, Dept Phys, 1110 West Green St, Urbana, IL USA.
[Bartolo, N.; Liguori, M.; Matarrese, S.] Univ Padua, Dipartimento Fis & Astron G Galilei, Via Marzolo 8, I-35131 Padua, Italy.
[Burigana, C.; Lattanzi, M.; Mandolesi, N.; Natoli, P.] Univ Ferrara, Dipartimento Fis & Sci Terra, Via Saragat 1, I-44122 Ferrara, Italy.
[de Bernardis, P.; Masi, S.; Melchiorri, A.; Pagano, L.; Piacentini, F.] Univ Roma La Sapienza, Dipartimento Fis, Ple A Moro 2, Rome, Italy.
[Bersanelli, M.; Maino, D.; Mennella, A.; Rossetti, M.; Tomasi, M.] Univ Milan, Dipartimento Fis, Via Celoria, I-16 Milan, Italy.
[Gregorio, A.] Univ Trieste, Dipartimento Fis, Via A Valerio 2, Trieste, Italy.
[Mazzotta, P.] Univ Roma Tor Vergata, Dipartimento Fis, Via Ric Sci, I-1 Rome, Italy.
[Renzi, A.] Univ Roma Tor Vergata, Dipartimento Matemat, Via Ric Sci, I-1 Rome, Italy.
[Christensen, P. R.; Naselsky, P.] Niels Bohr Inst, Discovery Ctr, Blegdamsvej 17, Copenhagen, Denmark.
[Rebolo, R.; Rubino-Martin, J. A.] Univ La Laguna, Dpto Astrofis, E-38206 Tenerife, Spain.
[Dupac, X.; Leonardi, R.; Lopez-Caniego, M.; Mendes, L.] Planck Sci Off, ESAC, European Space Agcy, Caminobajo Castillo S-N, Madrid 28692, Spain.
[Tauber, J. A.] ESTEC, European Space Agcy, Keplerlaan 1, NL-2201 AZ Noordwijk, Netherlands.
[Tcrcnzi, L.] Univ Studi E Campus, Fac Ingn, Via Isimbardi 10, I-22060 Novedrate, CO, Italy.
[Matarrese, S.] Ist Nazl Fis Nucl, Gran Sasso Sci Inst, Viale F Crispi 7, I-67100 Laquila, Italy.
[Pettorino, V.] HGSFP, Philosophenweg 16, D-69120 Heidelberg, Germany.
[Pettorino, V.] Heidelberg Univ, Dept Theoret Phys, Philosophenweg 16, D-69120 Heidelberg, Germany.
[Kurki-Suonio, H.; Savelainen, M.; Suur-Uski, A. S.; Valiviita, J.] Univ Helsinki, Helsinki Inst Phys, Gustaf Hallstromin Katu 2, Helsinki, Finland.
[Umana, G.] Osserv Astrofis Catania, INAF, Via S Sofia 78, Catania, Italy.
[de Zotti, G.] Osserv Astron Padova, INAF, Vicolo Osservatorio 5, Padua, Italy.
[Polcnta, G.] Osserv Astron Roma, INAF, Via Frascati 33, Monte Porzio Catone, Italy.
[Frailis, M.; Galeotta, S.; Gregorio, A.; Maggio, G.; Pasian, F.; Zacchei, A.] Osserv Astron Trieste, INAF, Via GB Tiepolo 11, Trieste, Italy.
[Burigana, C.; Butler, R. C.; Cuttaia, F.; de Rosa, A.; Finelli, F.; Franceschi, E.; Gruppuso, A.; Mandolesi, N.; Morgante, G.; Natoli, P.; Paoletti, D.; Sandri, M.; Tcrcnzi, L.; Toffolatti, L.; Valcnziano, L.; Villa, F.] INAF IASF Bologna, Via Gobetti 101, Bologna, Italy.
[Bersanelli, M.; Donzelli, S.; Maino, D.; Mennella, A.; Rossetti, M.; Tomasi, M.] INAF IASF Milano, Via E Bassini 15, Milan, Italy.
[Burigana, C.; Finelli, F.; Paoletti, D.] Ist Nazl Fis Nucl, Sez Bologna, Via Irnerio 46, I-40126 Bologna, Italy.
[Melchiorri, A.; Pagano, L.] Univ Roma Sapienza, Ist Nazl Fis Nucl, Sez Roma 1, Piazzale Aldo Moro 2, I-00185 Rome, Italy.
[Renzi, A.] Univ Roma Tor Vergata, Ist Nazl Fis Nucl, Sez Roma 2, Via Ric Sci 1, Rome, Italy.
[Gregorio, A.] Ist Nazl Fis Nucl, Natl Inst Nucl Phys, Via Valerio 2, I-34127 Trieste, Italy.
[Desert, F. X.] Univ Grenoble Alpes, Inst Planetol & Astrophys Grenoble, IPAG, CNRS, F-38000 Grenoble, France.
[Mitra, S.] IUCAA, Post Bag 4,Pune Univ Campus, Pune 411007, Maharashtra, India.
[Clements, D. L.; Ducout, A.; Jaffe, A. H.; Mortlock, D.] Imperial Coll London, Astrophys Grp, Blackett Lab, Prince Consort Rd, London SW7 2AZ, England.
[McGehee, P.; Paladini, R.; Pearson, T. J.; Pelkonen, V. M.; Rusholme, B.] CALTECH, Ctr Infrared Proc & Anal, Pasadena, CA 91125 USA.
[Benoit, A.] Univ Joseph Fourier Grenoble 1, CNRS, Inst Neel, 25 Rue Martyrs, Grenoble, France.
[Dole, H.] Inst Univ France, 103 Bd St Michel, F-75005 Paris, France.
[Aghanim, N.; Aumont, J.; Boulanger, F.; Chamballu, A.; Dole, H.; Douspis, M.; Hurier, G.; Kunz, M.; Mangilli, A.; Miville-Deschenes, M. A.; Pajot, F.; Pugct, J. L.; Remazeilles, M.] Univ Paris Sud 11, Inst Astrophys Spatiale, CNRS, UMR 8617, Batiment 121, Orsay, France.
[Benabed, K.; Benoit-Levy, A.; Bouchet, F. R.; Colombi, S.; Ducout, A.; Elsner, F.; Galli, S.; Hivon, E.; Moneti, A.; Prunct, S.; Sygnet, J. F.; Wandelt, B. D.] CNRS, Inst Astrophys Paris, UMR 7095, 98 Bis Blvd Arago, F-75014 Paris, France.
[Efstathiou, G.; Gratton, S.; Harrison, D. L.; Migliaccio, M.; Sutton, D.] Univ Cambridge, Inst Astron, Madingley Rd, Cambridge CB3 0HA, England.
[Eriksen, H. K.; Gjerlow, E.; Hansen, F. K.; Lilje, P. B.] Univ Oslo, Inst Theoret Astrophys, N-0371 Oslo, Norway.
[Rebolo, R.; Rubino-Martin, J. A.] Inst Astrofis Canarias, C Via Lactea S-N, Tenerife 38205, Spain.
[Barreiro, R. B.; Bonavera, L.; Curto, A.; Diego, J. M.; Gonzalez-Nuevo, J.; Herranz, D.; Lopez-Caniego, M.; Martinez-Gonzalez, E.; Toffolatti, L.; Vielva, P.] Univ Cantabria, CSIC, Inst Fis Cantabria, Avda Castros S-N, Santander, Spain.
[Bartolo, N.; Liguori, M.; Matarrese, S.] Ist Nazl Fis Nucl, Sez Padova, Via Marzolo 8, I-35131 Padua, Italy.
[Colombo, L. P. L.; Crill, B. P.; Dore, O.; Gorski, K. M.; Hanson, D.; Hildebrandt, S. R.; Holmes, W. A.; Lawrence, C. R.; Mitra, S.; Pietrobon, D.; Prczcau, G.; Rocha, G.; Roudier, G.; Seiffert, M. D.; Wade, L. A.; Wehus, I. K.] CALTECH, Jet Prop Lab, 4800 Oak Grove Dr, Pasadena, CA USA.
[Bonaldi, A.; Davies, R. D.; Davis, R. J.; Dickinson, C.; Noviello, F.; Remazeilles, M.] Univ Manchester, Jodrell Bank Ctr Astrophys, Sch Phys & Astron, Alan Turing Bldg,Oxford Rd, Manchester M13 9PL, Lancs, England.
[Ashdow, M.; Gratton, S.; Harrison, D. L.; Lasenby, A.; Migliaccio, M.; Stolyarov, V.; Sutton, D.] Kavli Inst Cosmol Cambridge, Madingley Rd, Cambridge CB3 0HA, England.
[Couchot, F.; Henrot-Versille, S.; Mangilli, A.; Perdereau, O.; Plaszczynski, S.] Univ Paris 11, LAL, CNRS, IN2P3, Orsay, France.
[Lesgourgues, J.] Univ Savoie, LAPTh, CNRS, BP 110, F-74941 Annecy Le Vieux, France.
[Catalano, A.; Coulais, A.; Falgarone, E.; Lamarre, J. M.; Levrier, F.; Roudier, G.] Observ Paris, CNRS, LERMA, 61 Ave Observ, Paris, France.
[Arnaud, M.; Chamballu, A.; Marshall, D. J.; Pratt, G. W.] Univ Paris Diderot, CEA Saclay, CNRS, Lab AIM,IRFU,Serv Astrophys,CEA DSM, Bat 709, F-91191 Gif Sur Yvette, France.
[Catalano, A.; Combet, C.; Macias-Perez, J. F.; Perotto, L.; Renault, C.; Santos, D.] Univ Grenoble Alpes, Lab Phys Subatom & Cosmol, CNRS, IN2P3, 53 Rue Martyrs, F-38026 Grenoble, France.
[Van Tent, B.] Univ Paris Sud 11, Phys Theor Lab, Batiment 210, F-91405 Orsay, France.
[Van Tent, B.] CNRS, Batiment 210, F-91405 Orsay, France.
[Kisner, T. S.] Lawrence Berkeley Natl Lab, Berkeley, CA 94720 USA.
[Novikov, D.; Novikov, I.] Russian Acad Sci, Lebedev Phys Inst, Ctr Astro Space, 84-32 Profsoyuznaya St, Moscow 117997, Russia.
[Ensslin, T. A.; Hernandez-Monteagudo, C.; Hovest, W.; Knoche, J.; Rachcn, J. P.; Reinecke, M.; Sunyaev, R.] Max Planck Inst Astrophys, Karl Schwarzschild Str 1, D-85741 Garching, Germany.
[Hanson, D.] McGill Univ, McGill Phys, Ernest Rutherford Phys Bldg,3600 Rue Univ, Montreal, PQ H3A 2T8, Canada.
[Murphy, J. A.] Natl Univ Ireland, Dept Expt Phys, Maynooth, Kildare, Ireland.
[Christensen, P. R.; Frejsel, A.; Naselsky, P.; Novikov, I.] Niels Bohr Inst, Blegdamsvej 17, Copenhagen, Denmark.
[Savini, G.] UCL, Opt Sci Lab, Gower St, London, England.
[Lesgourgues, J.] Ecole Polytech Fed Lausanne, SB ITP LPPC, CH-1015 Lausanne, Switzerland.
[Baccigalupi, C.; Bielewicz, P.; Danese, L.; de Zotti, G.; Gonzalez-Nuevo, J.; Paci, F.; Perrotta, F.] SISSA, Astrophys Sect, Via Bonomea 265, I-34136 Trieste, Italy.
[Ade, P. A. R.; Munshi, D.; Spencer, L. D.; Sudiwala, R.] Cardiff Univ, Sch Phys & Astron, Queens Bldg, Cardiff CF24 3AA, S Glam, Wales.
[Moss, A.] Univ Nottingham, Sch Phys & Astron, Nottingham NG7 2RD, England.
[Bouchet, F. R.] Sorbonne Univ, UPMC, Inst Astrophys Paris, UMR7095, 98 Bis Blvd Arago, F-75014 Paris, France.
[Sunyaev, R.] Russian Acad Sci, Space Res Inst IKI, Profsoyuznaya Str 84-32, Moscow 117997, Russia.
[Borrill, J.] Univ Calif Berkeley, Space Sci Lab, Berkeley, CA 94720 USA.
[Stolyarov, V.] Russian Acad Sci, Special Astrophys Observ, Nizhnii Arkhyz 369167, Zelenchukskiy R, Russia.
[Calabrese, E.] Univ Oxford, Subdept Astrophys, Keble Rd, Oxford OX1 3RH, England.
[Lesgourgues, J.] CERN, Div Theory, PH TH, CH-1211 Geneva 23, Switzerland.
[Benabed, K.; Benoit-Levy, A.; Colombi, S.; Elsner, F.; Hivon, E.; Prunct, S.; Wandelt, B. D.] Univ Paris 06, UPMC, UMR 7095, 98 Bis Blvd Arago, F-75014 Paris, France.
[Banday, A. J.; Bernard, J. P.; Bielewicz, P.; Forni, O.; Giard, M.; Jaffe, T. R.; Montier, L.; Pointccoutcau, E.; Ristorcelli, I.] Univ Toulouse, UPS OMP, IRAP, F-31028 Toulouse 4, France.
[Rcach, W. T.] Univ Space Res Assoc, Stratospher Observ Infrared Astron, MS 232-11, Moffett Field, CA 94035 USA.
[Battaner, E.] Univ Granada, Dept Fis Teor & Cosmos, Fac Ciencias, E-18071 Granada, Spain.
[Battaner, E.] Univ Granada, Inst Carlos Fis Teor & Computac 1, Granada, Spain.
[Gorski, K. M.] Univ Warsaw Observ, Aleje Ujazdowskie 4, PL-00478 Warsaw, Poland.
RP Montier, L (reprint author), IRAP, CNRS, 9 Av Colonel Roche,BP 44346, F-112AP Toulouse 4, France.; Montier, L (reprint author), Univ Toulouse, UPS OMP, IRAP, F-31028 Toulouse 4, France.
EM Ludovic.Montier@irap.orap.eu
RI Barreiro, Rita Belen/N-5442-2014; Mazzotta, Pasquale/B-1225-2016;
bonavera, laura/E-9368-2017; Gonzalez-Nuevo, Joaquin/I-3562-2014;
Herranz, Diego/K-9143-2014; Colombo, Loris/J-2415-2016;
OI Valiviita, Jussi/0000-0001-6225-3693; Barreiro, Rita
Belen/0000-0002-6139-4272; Mazzotta, Pasquale/0000-0002-5411-1748;
bonavera, laura/0000-0001-8039-3876; Gonzalez-Nuevo,
Joaquin/0000-0003-1354-6822; Herranz, Diego/0000-0003-4540-1417;
Colombo, Loris/0000-0003-4572-7732; TERENZI, LUCA/0000-0001-9915-6379;
Stolyarov, Vladislav/0000-0001-8151-828X; Reach,
William/0000-0001-8362-4094; Hurier, Guillaume/0000-0002-1215-0706;
Kurki-Suonio, Hannu/0000-0002-4618-3063; Zacchei,
Andrea/0000-0003-0396-1192; Toffolatti, Luigi/0000-0003-2645-7386;
Lilje, Per/0000-0003-4324-7794; Paoletti, Daniela/0000-0003-4761-6147;
Nati, Federico/0000-0002-8307-5088; Savini, Giorgio/0000-0003-4449-9416;
Pierpaoli, Elena/0000-0002-7957-8993; Juvela, Mika/0000-0002-5809-4834
FU ESA; CNES (France); CNRS/INSU-IN2P3-INP (France); ASI (Italy); CNR
(Italy); INAF (Italy); NASA (USA); DoE (USA); STFC (UK); UKSA (UK); CSIC
(Spain); MINECO (Spain); J.A. (Spain); RES (Spain); Tekes (Finland); AoF
(Finland); CSC (Finland); DLR (Germany); MPG (Germany); CSA (Canada);
DTU Space (Denmark); SER/SSO (Switzerland); RCN (Norway); SFI (Ireland);
FCT/MCTES (Portugal); ERC (EU); PRACE (EU)
FX The Planck Collaboration acknowledges the support of: ESA; CNES and
CNRS/INSU-IN2P3-INP (France); ASI, CNR, and INAF (Italy); NASA and DoE
(USA); STFC and UKSA (UK); CSIC, MINECO, J.A.; and RES (Spain); Tekes,
AoF, and CSC (Finland); DLR and MPG (Germany); CSA (Canada); DTU Space
(Denmark); SER/SSO (Switzerland); RCN (Norway); SFI (Ireland); FCT/MCTES
(Portugal); ERC and PRACE (EU). A description of the Planck
Collaboration and a list of its members, indicating which technical or
scientific activities they have been involved in, can be found at
http://www.cosmos.esa.int/web/planck/planck-collaboration.
NR 112
TC 0
Z9 0
U1 1
U2 1
PU EDP SCIENCES S A
PI LES ULIS CEDEX A
PA 17, AVE DU HOGGAR, PA COURTABOEUF, BP 112, F-91944 LES ULIS CEDEX A,
FRANCE
SN 1432-0746
J9 ASTRON ASTROPHYS
JI Astron. Astrophys.
PD OCT
PY 2016
VL 594
AR A28
DI 10.1051/0004-6361/201525819
PG 28
WC Astronomy & Astrophysics
SC Astronomy & Astrophysics
GA DZ4MG
UT WOS:000385832200007
ER
PT J
AU Ade, PAR
Aghanim, N
Ashdown, M
Aumont, J
Baccigalupi, C
Ballardini, M
Banday, AJ
Barreiro, RB
Bartolo, N
Basak, S
Battaglia, P
Battaner, E
Benabed, K
Benoit, A
Benoit-Levy, A
Bernard, JP
Bersanelli, M
Bielewicz, P
Bock, JJ
Bonaldi, A
Bonavera, L
Bond, JR
Borrill, J
Bouchet, FR
Bucher, M
Burigana, C
Butler, RC
Calabrese, E
Cardoso, JF
Castex, G
Catalano, A
Chamballu, A
Christensen, PR
Colombi, S
Colombo, LPL
Crill, BP
Curto, A
Cuttaia, F
Danese, L
Davies, RD
Davis, RJ
de Bernardis, P
de Rosa, A
de Zotti, G
Delabrouille, J
Dickinson, C
Diego, JM
Dole, H
Donzelli, S
Dore, O
Douspis, M
Ducout, A
Dupac, X
Efstathiou, G
Elsner, F
Ensslin, TA
Eriksen, HK
Fergusson, J
Finelli, F
Forni, O
Frailis, M
Franceschet, C
Franceschi, E
Frejsel, A
Galeotta, S
Galli, S
Ganga, K
Giard, M
Giraud-Heraud, Y
Gjerlow, E
Gonzalez-Nuevo, J
Gorski, KM
Gratton, S
Gregorio, A
Gruppuso, A
Hansen, FK
Hanson, D
Harrison, DL
Henrot-Versille, S
Herranz, D
Hildebrandt, SR
Hivon, E
Hobson, M
Holmes, WA
Hornstrup, A
Hovest, W
Huffenberger, KM
Hurier, G
Jaffe, AH
Jaffe, TR
Juvela, M
Keihanen, E
Keskitalo, R
Kiiveri, K
Kisner, TS
Knoche, J
Krachmalnicoff, N
Kunz, M
Kurki-Suonio, H
Lagache, G
Lahteenmaki, A
Lamarre, JM
Lasenby, A
Lattanzi, M
Lawrence, CR
Leahy, JP
Leonardi, R
Lesgourgues', J
Levrier, F
Liguori, M
Lilje, PB
Linden-Vornle, M
Lindholm, V
Lopez-Caniego, M
Lubin, PM
Macias-Perez, JF
Maggio, G
Maino, D
Mandolesi, N
Mangilli, A
Maris, M
Martin, PG
Martinez-Gonzalez, E
Masi, S
Matarrese, S
Mazzotta, P
McGehee, P
Meinhold, PR
Melchiorri, A
Mendes, L
Mennella, A
Migliaccio, M
Mitra, S
Montier, L
Morgante, G
Morisset, N
Mortlock, D
Moss, A
Munshi, D
Murphy, JA
Naselsky, P
Nati, F
Natoli, P
Netterfield, CB
Norgaard-Nielsen, HU
Novikov, D
Novikov, I
Oppermann, N
Paci, F
Pagano, L
Paoletti, D
Partridge, B
Pasian, F
Patanchon, G
Pearson, TJ
Peel, M
Perdereau, O
Perotto, L
Perrotta, F
Pettorino, V
Piacentini, F
Pierpaoli, E
Pietrobon, D
Pointecouteau, E
Polenta, G
Pratt, GW
Prezeau, G
Prunet, S
Puget, JL
Rachen, JP
Rebolo, R
Reinecke, M
Remazeilles, M
Renzi, A
Rocha, G
Romelli, E
Rosset, C
Rossetti, M
Roudier, G
Rubino-Martin, JA
Rusholme, B
Sandri, M
Santos, D
Savelainen, M
Scott, D
Seiffert, MD
Shellard, EPS
Spencer, LD
Stolyarov, V
Sutton, D
Suur-Uski, AS
Sygnet, JF
Tauber, JA
Tavagnacco, D
Terenzi, L
Toffolatti, L
Tomasi, M
Tristram, M
Tucci, M
Tuovinen, J
Turler, M
Umana, G
Valenziano, L
Valiviita, J
Van Tent, B
Vassallo, T
Vielva, P
Villa, F
Wade, LA
Wandelt, BD
Watson, R
Wehus, IK
Wilkinson, A
Yvon, D
Zacchei, A
Zonca, A
AF Ade, P. A. R.
Aghanim, N.
Ashdown, M.
Aumont, J.
Baccigalupi, C.
Ballardini, M.
Banday, A. J.
Barreiro, R. B.
Bartolo, N.
Basak, S.
Battaglia, P.
Battaner, E.
Benabed, K.
Benoit, A.
Benoit-Levy, A.
Bernard, J. P.
Bersanelli, M.
Bielewicz, P.
Bock, J. J.
Bonaldi, A.
Bonavera, L.
Bond, J. R.
Borrill, J.
Bouchet, F. R.
Bucher, M.
Burigana, C.
Butler, R. C.
Calabrese, E.
Cardoso, J. F.
Castex, G.
Catalano, A.
Chamballu, A.
Christensen, P. R.
Colombi, S.
Colombo, L. P. L.
Crill, B. P.
Curto, A.
Cuttaia, F.
Danese, L.
Davies, R. D.
Davis, R. J.
de Bernardis, P.
de Rosa, A.
de Zotti, G.
Delabrouille, J.
Dickinson, C.
Diego, J. M.
Dole, H.
Donzelli, S.
Dore, O.
Douspis, M.
Ducout, A.
Dupac, X.
Efstathiou, G.
Elsner, F.
Ensslin, T. A.
Eriksen, H. K.
Fergusson, J.
Finelli, F.
Forni, O.
Frailis, M.
Franceschet, C.
Franceschi, E.
Frejsel, A.
Galeotta, S.
Galli, S.
Ganga, K.
Giard, M.
Giraud-Heraud, Y.
Gjerlow, E.
Gonzalez-Nuevo, J.
Gorski, K. M.
Gratton, S.
Gregorio, A.
Gruppuso, A.
Hansen, F. K.
Hanson, D.
Harrison, D. L.
Henrot-Versille, S.
Herranz, D.
Hildebrandt, S. R.
Hivon, E.
Hobson, M.
Holmes, W. A.
Hornstrup, A.
Hovest, W.
Huffenberger, K. M.
Hurier, G.
Jaffe, A. H.
Jaffe, T. R.
Juvela, M.
Keihanen, E.
Keskitalo, R.
Kiiveri, K.
Kisner, T. S.
Knoche, J.
Krachmalnicoff, N.
Kunz, M.
Kurki-Suonio, H.
Lagache, G.
Lahteenmaki, A.
Lamarre, J. M.
Lasenby, A.
Lattanzi, M.
Lawrence, C. R.
Leahy, J. P.
Leonardi, R.
Lesgourgues, J.
Levrier, F.
Liguori, M.
Lilje, P. B.
Linden-Vornle, M.
Lindholm, V.
Lopez-Caniego, M.
Lubin, P. M.
Macias-Perez, J. F.
Maggio, G.
Maino, D.
Mandolesi, N.
Mangilli, A.
Maris, M.
Martin, P. G.
Martinez-Gonzalez, E.
Masi, S.
Matarrese, S.
Mazzotta, P.
McGehee, P.
Meinhold, P. R.
Melchiorri, A.
Mendes, L.
Mennella, A.
Migliaccio, M.
Mitra, S.
Montier, L.
Morgante, G.
Morisset, N.
Mortlock, D.
Moss, A.
Munshi, D.
Murphy, J. A.
Naselsky, P.
Nati, F.
Natoli, P.
Netterfield, C. B.
Norgaard-Nielsen, H. U.
Novikov, D.
Novikov, I.
Oppermann, N.
Paci, F.
Pagano, L.
Paoletti, D.
Partridge, B.
Pasian, F.
Patanchon, G.
Pearson, T. J.
Peel, M.
Perdereau, O.
Perotto, L.
Perrotta, F.
Pettorino, V.
Piacentini, F.
Pierpaoli, E.
Pietrobon, D.
Pointecouteau, E.
Polenta, G.
Pratt, G. W.
Prezeau, G.
Prunet, S.
Puget, J. L.
Rachen, J. P.
Rebolo, R.
Reinecke, M.
Remazeilles, M.
Renzi, A.
Rocha, G.
Romelli, E.
Rosset, C.
Rossetti, M.
Roudier, G.
Rubino-Martin, J. A.
Rusholme, B.
Sandri, M.
Santos, D.
Savelainen, M.
Scott, D.
Seiffert, M. D.
Shellard, E. P. S.
Spencer, L. D.
Stolyarov, V.
Sutton, D.
Suur-Uski, A. S.
Sygnet, J. F.
Tauber, J. A.
Tavagnacco, D.
Terenzi, L.
Toffolatti, L.
Tomasi, M.
Tristram, M.
Tucci, M.
Tuovinen, J.
Turler, M.
Umana, G.
Valenziano, L.
Valiviita, J.
Van Tent, B.
Vassallo, T.
Vielva, P.
Villa, F.
Wade, L. A.
Wandelt, B. D.
Watson, R.
Wehus, I. K.
Wilkinson, A.
Yvon, D.
Zacchei, A.
Zonca, A.
CA Planck Collaboration
TI Planck 2015 results II. Low Frequency Instrument data processings
SO ASTRONOMY & ASTROPHYSICS
LA English
DT Article
DE space vehicles: instruments; methods: data analysis; cosmic background
radiation
ID PRE-LAUNCH STATUS; POWER SPECTRUM; DATA SETS; MICROWAVE; MADAM; MAPS
AB We present an updated description of the Planck Low Frequency Instrument (LFI) data processing pipeline, associated with the 2015 data release. We point out the places where our results and methods have remained unchanged since the 2013 paper and we highlight the changes made for the 2015 release, describing the products (especially timelines) and the ways in which they were obtained. We demonstrate that the pipeline is self-consistent (principally based on simulations) and report all null tests. For the first time, we present LFI maps in Stokes Q and U polarization. We refer to other related papers where more detailed descriptions of the LFI data processing pipeline may be found if needed.
C1 [Bucher, M.; Cardoso, J. F.; Castex, G.; Curto, A.; Delabrouille, J.; Ganga, K.; Giraud-Heraud, Y.; Patanchon, G.; Rosset, C.; Roudier, G.] Univ Paris Diderot, CNRS, Sorbonne Paris Cite,Observ Paris, APC,AstroParticule & Cosmol,IN2P3,CEA,Lrfu, 10 Rue Alice Domon & Leonie Duquet, F-75205 Paris 13, France.
[Lahteenmaki, A.] Aalto Univ, Metsahovi Radio Observ, POB 13000, Aalto 00076, Finland.
[Lahteenmaki, A.] Dept Radio Sci & Engn, POB 13000, Aalto 00076, Finland.
[Kunz, M.] African Inst Math Sci, 6-8 Melrose Rd, Cape Town, South Africa.
[Natoli, P.; Polenta, G.] Agenzia Spaziale Italiana Sci, Ctr Data, Via Politecn Snc, I-00133 Rome, Italy.
[Lagache, G.] Aix Marseille Univ, CNRS, LAM, UMR 7326, F-13388 Marseille, France.
[Ashdown, M.; Curto, A.; Hobson, M.; Lasenby, A.; Stolyarov, V.] Univ Cambridge, Cavendish Lab, Astrophys Grp, J J Thomson Ave, Cambridge CB3 OHE, England.
[Leonardi, R.] CGEE, SCS Qd 9,Lote C,Torre C,4 Andar, BR-70308200 Brasilia, DF, Brazil.
[Bond, J. R.; Hanson, D.; Martin, P. G.; Oppermann, N.] Univ Toronto, CITA, 60 St George St, Toronto, ON M5S 3H8, Canada.
[Banday, A. J.; Bernard, J. P.; Bielewicz, P.; Forni, O.; Giard, M.; Jaffe, T. R.; Montier, L.; Pointecouteau, E.] IRAP, CNRS, 9 Av Colonel Roche,BP 44346, F-31028 Toulouse 4, France.
[Tuovinen, J.] Trinity Coll Dublin, CRANN, Dublin, Ireland.
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[Fergusson, J.; Shellard, E. P. S.] Univ Cambridge, Ctr Theoret Cosmol, Wilberforce Rd, Cambridge CB3 0WA, England.
[Borrill, J.; Keskitalo, R.] Lawrence Berkeley Natl Lab, Computat Cosmol Ctr, 1 Cyclotron Rd, Berkeley, CA 94720 USA.
[Rebolo, R.] CSIC, Calle Serrano 117, Madrid 28006, Spain.
[Chamballu, A.; Yvon, D.] CEA Saclay, DSM, Irfu, SPP, F-91191 Gif Sur Yvette, France.
[Hornstrup, A.; Linden-Vornle, M.; Norgaard-Nielsen, H. U.] Tech Univ Denmark, Natl Space Inst, DTU Space, Elektrovej 327, DK-2800 Lyngby, Denmark.
[Kunz, M.; Tucci, M.] Univ Geneva, Dept Phys Theor, 24 Quai E Ansermet, CH-1211 Geneva 4, Switzerland.
[Rebolo, R.; Rubino-Martin, J. A.] Univ La Laguna, Dept Astrofis, E-38206 Tenerife, Spain.
[Gonzalez-Nuevo, J.; Toffolatti, L.] Univ Oviedo, Dept Fis, Avda Calvo Sotelo S-N, E-33007 Oviedo, Spain.
[Netterfield, C. B.] Univ Toronto, Dept Astron & Astrophys, 50 St George St, Toronto, ON M5S 3H4, Canada.
[Rachen, J. P.] Radboud Univ Nijmegen, Dept Astrophys IMAPP, POB 9010, NL-6500 GL Nijmegen, Netherlands.
[Scott, D.] Univ British Columbia, Dept Phys & Astron, 6224 Agr Rd, Vancouver, BC V6T 1Z1, Canada.
[Colombo, L. P. L.; Pierpaoli, E.] Univ Southern Calif, Dept Phys & Astron, Dana & David Dornsife Coll Letter Arts & Sci, Los Angeles, CA 90089 USA.
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[Battaglia, P.; de Bernardis, P.; Masi, S.; Melchiorri, A.; Pagano, L.; Piacentini, F.] Univ Roma La Sapienza, Dipartimento Fis, Ple A Moro 2, I-00185 Rome, Italy.
[Bersanelli, M.; Franceschet, C.; Krachmalnicoff, N.; Maino, D.; Mennella, A.; Rossetti, M.; Tomasi, M.] Univ Milan, Dipartimento Fis, Via Celoria 16, I-20133 Milan, Italy.
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[Christensen, P. R.] Niels Bohr Inst, Discovery Ctr, Blegdamsvej 17, DK-2100 Copenhagen, Denmark.
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[Pettorino, V.] HGSFP, Philosophenweg 16, D-69120 Heidelberg, Germany.
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[Partridge, B.] Haverford Coll, Dept Astron, 370 Lancaster Ave, Haverford, PA 19041 USA.
[Kiiveri, K.; Kurki-Suonio, H.; Lahteenmaki, A.; Lindholm, V.; Savelainen, M.; Suur-Uski, A. S.; Valiviita, J.] Univ Helsinki, Helsinki Inst Phys, Gustaf Hallstromin Katu 2, FIN-00014 Helsinki, Finland.
[Umana, G.] Osserv Astrofis Catania, INAF, Via S Sofia 78, I-95123 Catania, Italy.
[de Zotti, G.] Osserv Astron Padova, INAF, Vicolo Osservatorio 5, I-35122 Padua, Italy.
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[Ballardini, M.; Burigana, C.; Finelli, F.; Paoletti, D.] Ist Nazl Fis Nucl, Sez Bologna, Via Irnerio 46, I-40126 Bologna, Italy.
[Melchiorri, A.; Pagano, L.] Univ Roma Sapienza, Ist Nazl Fis Nucl, Sez Roma 1, Ple Aldo Moro 2, I-00185 Rome, Italy.
[Renzi, A.] Univ Roma Tor Vergata, Ist Nazl Fis Nucl, Sez Roma 2, Via Ric Sci 1, I-00133 Rome, Italy.
[Gregorio, A.] Ist Nazl Fis Nucl, Natl Inst Nucl Phys, Via Valerio 2, I-34127 Trieste, Italy.
[Morisset, N.; Turler, M.] Univ Geneva, Dept Astron, ISDC, Ch Ecogia 16, CH-1290 Versoix, Switzerland.
[Mitra, S.] IUCAA, Post Bag 4,Pune Univ Campus, Pune 411007, Maharashtra, India.
[Ducout, A.; Jaffe, A. H.; Mortlock, D.] Imperial Coll London, Astrophys Grp, Blackett Lab, Prince Consort Rd, London SW7 2AZ, England.
[McGehee, P.; Pearson, T. J.; Rusholme, B.] CALTECH, Ctr Infrared Proc & Anal, Pasadena, CA 91125 USA.
[Benoit, A.] Univ Joseph Fourier Grenoble 1, CNRS, Inst Neel, 25 Rue Martyrs, F-38042 Grenoble, France.
[Dole, H.] Inst Univ France, 103 Bd St Michel, F-75005 Paris, France.
[Aghanim, N.; Aumont, J.; Chamballu, A.; Dole, H.; Douspis, M.; Hurier, G.; Kunz, M.; Lagache, G.; Mangilli, A.; Puget, J. L.; Remazeilles, M.] Univ Paris Saclay, Univ Paris Sud, CNRS, Inst Astrophys Spatiale, Bat 121, F-91405 Orsay, France.
[Benabed, K.; Benoit-Levy, A.; Bouchet, F. R.; Cardoso, J. F.; Colombi, S.; Ducout, A.; Elsner, F.; Hivon, E.; Prunet, S.; Sygnet, J. F.; Wandelt, B. D.] CNRS, Inst Astrophys Paris, UMR 7095, 98 Bis Blvd Arago, F-75014 Paris, France.
[Lesgourgues, J.] Rhein Westfal TH Aachen, Inst Theoret Teilchenphys & Kosmol, D-52056 Aachen, Germany.
[Efstathiou, G.; Gratton, S.; Harrison, D. L.; Migliaccio, M.; Sutton, D.] Univ Cambridge, Inst Astron, Madingley Rd, Cambridge CB3 0HA, England.
[Eriksen, H. K.; Gjerlow, E.; Hansen, F. K.; Lilje, P. B.; Wehus, I. K.] Univ Oslo, Inst Theoret Astrophys, POB 1029, N-0315 Oslo, Norway.
[Rebolo, R.; Rubino-Martin, J. A.] Inst Astrofis Canarias, C Via Lactea S-N, Tenerife 38205, Spain.
[Barreiro, R. B.; Bonavera, L.; Curto, A.; Diego, J. M.; Gonzalez-Nuevo, J.; Herranz, D.; Lopez-Caniego, M.; Martinez-Gonzalez, E.; Toffolatti, L.; Vielva, P.] Univ Cantabria, CSIC, Inst Fis Cantabria, Avda Castros S-N, E-39005 Santander, Spain.
[Bartolo, N.; Liguori, M.; Matarrese, S.] Ist Nazl Fis Nucl, Sez Padova, Via Marzolo 8, I-35131 Padua, Italy.
[Bock, J. J.; Colombo, L. P. L.; Crill, B. P.; Dore, O.; Gorski, K. M.; Hanson, D.; Hildebrandt, S. R.; Holmes, W. A.; Lawrence, C. R.; Mitra, S.; Pietrobon, D.; Prezeau, G.; Rocha, G.; Roudier, G.; Seiffert, M. D.; Wade, L. A.; Wehus, I. K.] CALTECH, Jet Prop Lab, 4800 Oak Grove Dr, Pasadena, CA 91109 USA.
[Bonaldi, A.; Davies, R. D.; Davis, R. J.; Dickinson, C.; Leahy, J. P.; Peel, M.; Remazeilles, M.; Watson, R.; Wilkinson, A.] Univ Manchester, Jodrell Bank Ctr Astrophys, Sch Phys & Astron, Alan Turing Bldg,Oxford Rd, Manchester M13 9PL, Lancs, England.
[Galli, S.] Univ Chicago, Kavli Inst Cosmol Phys, Chicago, IL 60637 USA.
[Ashdown, M.; Curto, A.; Gratton, S.; Harrison, D. L.; Lasenby, A.; Migliaccio, M.; Sutton, D.] Kavli Inst Cosmol Cambridge, Madingley Rd, Cambridge CB3 0HA, England.
[Stolyarov, V.] Kazan Fed Univ, 18 Kremlyovskaya St, Kazan 420008, Russia.
[Henrot-Versille, S.; Mangilli, A.; Perdereau, O.; Tristram, M.] Univ Paris 11, LAL, CNRS, IN2P3, F-91898 Orsay, France.
[Catalano, A.; Lamarre, J. M.; Levrier, F.; Roudier, G.] CNRS, Observ Paris, LERMA, 61 Ave Observ, F-75014 Paris, France.
[Chamballu, A.; Pratt, G. W.] Univ Paris Diderot, CEA Saclay, CNRS, Lab AIM,IRFU,Serv Astrophys,CEA DSM, Bat 709, F-91191 Gif Sur Yvette, France.
[Cardoso, J. F.] CNRS, Lab Traitement & Commun Informat, UMR 5141, 46 Rue Barrault, F-75634 Paris 13, France.
[Cardoso, J. F.] Telecom ParisTech, 46 Rue Barrault, F-75634 Paris 13, France.
[Catalano, A.; Macias-Perez, J. F.; Perotto, L.; Santos, D.] Univ Grenoble Alpes, Lab Phys Subatom & Cosmol, CNRS, IN2P3, 53 Rue Martyrs, F-38026 Grenoble, France.
[Van Tent, B.] Univ Paris Sud 11, Phys Theor Lab, Batiment 210, F-91405 Orsay, France.
[Van Tent, B.] CNRS, Batiment 210, F-91405 Orsay, France.
[Kisner, T. S.] Lawrence Berkeley Natl Lab, Berkeley, CA 94720 USA.
[Novikov, D.; Novikov, I.] Russian Acad Sci, Lebedev Phys Inst, Ctr Astro Space, 84-32 Profsoyuznaya St,GSP 7, Moscow 117997, Russia.
[Ensslin, T. A.; Hovest, W.; Knoche, J.; Rachen, J. P.; Reinecke, M.] Max Planck Inst Astrophys, Karl Schwarzschild Str 1, D-85741 Garching, Germany.
[Hanson, D.] McGill Univ, McGill Phys, Ernest Rutherford Phys Bldg,3600 Rue Univ, Montreal, PQ H3A 2T8, Canada.
[Murphy, J. A.] Natl Univ Ireland, Dept Expt Phys, Maynooth, Kildare, Ireland.
[Bielewicz, P.] Nicolaus Copernicus Astron Ctr, Bartycka 18, PL-00716 Warsaw, Poland.
[Christensen, P. R.; Frejsel, A.; Novikov, I.] Niels Bohr Inst, Blegdamsvej 17, DK-2100 Copenhagen, Denmark.
[Naselsky, P.] Univ Copenhagen, Niels Bohr Inst, Blegdamsvej 17, DK-2100 Copenhagen, Denmark.
[Baccigalupi, C.; Basak, S.; Bielewicz, P.; Danese, L.; de Zotti, G.; Paci, F.; Perrotta, F.] SISSA, Astrophys Sect, Via Bonomea 265, I-34136 Trieste, Italy.
[Terenzi, L.] Univ E Campus, SMARTEST Res Ctr, Via Isimbardi 10, I-22060 Novedrate, CO, Italy.
[Ade, P. A. R.; Munshi, D.; Spencer, L. D.] Cardiff Univ, Sch Phys & Astron, Queens Bldg, Cardiff CF24 3AA, S Glam, Wales.
[Moss, A.] Univ Nottingham, Sch Phys & Astron, Nottingham NG7 2RD, England.
[Bouchet, F. R.] Sorbonne Univ, UPMC, Inst Astrophys Paris, UMR 7095, 98 Bis Blvd Arago, F-75014 Paris, France.
[Borrill, J.] Univ Calif Berkeley, Space Sci Lab, Berkeley, CA 94720 USA.
[Stolyarov, V.] Russian Acad Sci, Special Astrophys Observ, Nizhnii Arkhyz 369167, Zelenchukskiy R, Russia.
[Calabrese, E.] Univ Oxford, Subdept Astrophys, Keble Rd, Oxford OX1 3RH, England.
[Lesgourgues, J.] CERN, Div Theory, PH TH, CH-1211 Geneva 23, Switzerland.
[Benabed, K.; Benoit-Levy, A.; Colombi, S.; Elsner, F.; Hivon, E.; Prunet, S.; Wandelt, B. D.] Univ Paris 06, UPMC, UMR 7095, 98 Bis Blvd Arago, F-75014 Paris, France.
[Banday, A. J.; Bernard, J. P.; Forni, O.; Giard, M.; Jaffe, T. R.; Montier, L.; Pointecouteau, E.] Univ Toulouse, UPS OMP, IRAP, F-31028 Toulouse 4, France.
[Battaner, E.] Univ Granada, Fac Ciencias, Dept Fis Teor & Cosmos, Granada 18003, Spain.
[Battaner, E.] Univ Granada, Inst Carlos Fis Teor & Comp 1, E-18071 Granada, Spain.
[Gorski, K. M.] Univ Warsaw Observ, Aleje Ujazdowskie 4, PL-00478 Warsaw, Poland.
RP Zacchei, A (reprint author), Osserv Astron Trieste, INAF, Via GB Tiepolo 11, I-34143 Trieste, Italy.
EM zacchei@oats.inaf.it
RI Lahteenmaki, Anne/L-5987-2013; Barreiro, Rita Belen/N-5442-2014;
Mazzotta, Pasquale/B-1225-2016; bonavera, laura/E-9368-2017;
Gonzalez-Nuevo, Joaquin/I-3562-2014; Herranz, Diego/K-9143-2014;
Colombo, Loris/J-2415-2016;
OI TERENZI, LUCA/0000-0001-9915-6379; Valiviita, Jussi/0000-0001-6225-3693;
Piacentini, Francesco/0000-0002-5444-9327; Nati,
Federico/0000-0002-8307-5088; Pierpaoli, Elena/0000-0002-7957-8993;
Juvela, Mika/0000-0002-5809-4834; Paoletti, Daniela/0000-0003-4761-6147;
Barreiro, Rita Belen/0000-0002-6139-4272; Mazzotta,
Pasquale/0000-0002-5411-1748; bonavera, laura/0000-0001-8039-3876;
Gonzalez-Nuevo, Joaquin/0000-0003-1354-6822; Herranz,
Diego/0000-0003-4540-1417; Colombo, Loris/0000-0003-4572-7732;
Kurki-Suonio, Hannu/0000-0002-4618-3063; Zacchei,
Andrea/0000-0003-0396-1192; Stolyarov, Vladislav/0000-0001-8151-828X
FU ESA; CNES (France); CNRS/INSU-IN2P3-INP (France); ASI (Italy); CNR
(Italy); INAF (Italy); NASA (USA); DoE (USA); STFC (UK); UKSA (UK); CSIC
(Spain); MINECO (Spain); JA (Spain); RES (Spain); Tekes (Finland); AoF
(Finland); CSC (Finland); DLR (Germany); MPG (Germany); CSA (Canada);
DTU Space (Denmark); SER/SSO (Switzerland); RCN (Norway); SFI (Ireland);
FCT/MCTES (Portugal); ERC (EU); PRACE (EU)
FX The Planck Collaboration acknowledges the support of: ESA; CNES and
CNRS/INSU-IN2P3-INP (France); ASI, CNR, and INAF (Italy); NASA and DoE
(USA); STFC and UKSA (UK); CSIC, MINECO, JA, and RES (Spain); Tekes,
AoF, and CSC (Finland); DLR and MPG (Germany); CSA (Canada); DTU Space
(Denmark); SER/SSO (Switzerland); RCN (Norway); SFI (Ireland); FCT/MCTES
(Portugal); ERC and PRACE (EU). A description of the Planck
Collaboration and a list of its members, indicating which technical or
scientific activities they have been involved in, can be found at
http://www.cosmos.esa.et/web/planck/. Finally, we thank Benjamin Walter
for a careful reading of the manuscript.
NR 58
TC 1
Z9 1
U1 1
U2 1
PU EDP SCIENCES S A
PI LES ULIS CEDEX A
PA 17, AVE DU HOGGAR, PA COURTABOEUF, BP 112, F-91944 LES ULIS CEDEX A,
FRANCE
SN 1432-0746
J9 ASTRON ASTROPHYS
JI Astron. Astrophys.
PD OCT
PY 2016
VL 594
AR A2
DI 10.1051/0004-6361/201525818
PG 35
WC Astronomy & Astrophysics
SC Astronomy & Astrophysics
GA DZ4MG
UT WOS:000385832200006
ER
PT J
AU Ade, PAR
Aghanim, N
Ashdown, M
Aumont, J
Baccigalupi, C
Banday, AJ
Barreiro, RB
Bartolo, N
Battaner, E
Benabed, K
Benoit, A
Benoit-Levy, A
Bernard, JP
Bersanelli, M
Bielewic, P
Bonaldi, A
Bonavera, L
Bond, JR
Borrill, J
Bouchet, FR
Bucher, M
Burigana, C
Butler, RC
Calabrese, E
Cardoso, JF
Catalano, A
Chamballu, A
Chary, RR
Christensen, PR
Colombi, S
Colombo, LPL
Crill, BP
Curto, A
Cuttaia, F
Danese, L
Davies, RD
Davis, RJ
de Bernardis, P
de Rosa, A
de Zotti, G
Delabrouille, J
Dickinson, C
Diego, JM
Dole, H
Donzelli, S
Dore, O
Douspis, M
Ducout, A
Dupac, X
Efstathiou, G
Elsner, F
Ensslin, TA
Eriksen, HK
Fergusson, J
Finelli, F
Forni, O
Frailis, M
Franceschi, E
Frejsel, A
Galeotta, S
Galli, S
Ganga, K
Giard, M
Giraud-Heraud, Y
Gjerlow, E
Gonzalez-Nuevo, J
Gorski, KM
Gratton, S
Gregorio, A
Gruppuso, A
Hansen, FK
Hanson, D
Harrison, DL
Henrot-Versille, S
Herranz, D
Hildebrandt, SR
Hivon, E
Hobson, M
Holmes, WA
Hornstrup, A
Hovest, W
Huffenberger, KM
Hurier, G
Jaffe, AH
Jaffe, TR
Juvela, M
Keihanen, E
Keskitalo, R
Kiiveri, K
Kisner, TS
Knoche, J
Kunz, M
Kurki-Suonio, H
Lahteenmaki, A
Lamarre, JM
Lasenby, A
Lattanzi, M
Lawrence, CR
Leahy, JP
Leonardi, R
Lesgourgues, J
Levrier, F
Liguori, M
Lilje, PB
Linden-Vornle, M
Lindholm, V
Lopez-Caniego, M
Lubin, PM
Macias-Perez, JF
Maggio, G
Maino, D
Mandolesi, N
Mangilli, A
Martin, PG
Martinez-Gonzalez, E
Masi, S
Matarrese, S
Mazzotta, P
McGehee, P
Meinhold, PR
Melchiorri, A
Mendes, L
Mennella, A
Migliaccio, M
Mitra, S
Montier, L
Morgante, G
Mortlock, D
Moss, A
Munshi, D
Murphy, JA
Naselsky, P
Nati, F
Natoli, P
Netterfield, CB
Norgaard-Nielsen, HU
Novikov, D
Novikov, I
Paci, F
Pagano, L
Paoletti, D
Partridge, B
Pasian, F
Patanchon, G
Pearson, TJ
Perdereau, O
Perotto, L
Perrotta, F
Pettorino, V
Pierpaoli, E
Pietrobon, D
Pointecouteau, E
Polenta, G
Pratt, GW
Prezeau, G
Prunet, S
Puget, JL
Rachen, JP
Rebolo, R
Reinecke, M
Remazeilles, M
Renzi, A
Rocha, G
Rosset, C
Rossetti, M
Roudier, G
Rubino-Martin, JA
Rusholme, B
Sandri, M
Santos, D
Savelainen, M
Scott, D
Seiffert, MD
Shellard, EPS
Spencer, LD
Stolyarov, V
Stompor, R
Sutton, D
Suur-Uski, AS
Sygnet, JF
Tauber, JA
Terenzi, L
Toffolatti, L
Tomasi, M
Tristram, M
Tucci, M
Tuovinen, J
Valenziano, L
Valiviita, J
Van Tent, B
Vassallo, T
Vielva, P
Villa, F
Wade, LA
Wandelt, BD
Watson, R
Wehus, IK
Yvon, D
Zacchei, A
Zonca, A
AF Ade, P. A. R.
Aghanim, N.
Ashdown, M.
Aumont, J.
Baccigalupi, C.
Banday, A. J.
Barreiro, R. B.
Bartolo, N.
Battaner, E.
Benabed, K.
Benoit, A.
Benoit-Levy, A.
Bernard, J. -P.
Bersanelli, M.
Bielewic, P.
Bonaldi, A.
Bonavera, L.
Bond, J. R.
Borrill, J.
Bouchet, F. R.
Bucher, M.
Burigana, C.
Butler, R. C.
Calabrese, E.
Cardoso, J. -F.
Catalano, A.
Chamballu, A.
Chary, R. -R.
Christensen, P. R.
Colombi, S.
Colombo, L. P. L.
Crill, B. P.
Curto, A.
Cuttaia, F.
Danese, L.
Davies, R. D.
Davis, R. J.
de Bernardis, P.
de Rosa, A.
de Zotti, G.
Delabrouille, J.
Dickinson, C.
Diego, J. M.
Dole, H.
Donzelli, S.
Dore, O.
Douspis, M.
Ducout, A.
Dupac, X.
Efstathiou, G.
Elsner, F.
Ensslin, T. A.
Eriksen, H. K.
Fergusson, J.
Finelli, F.
Forni, O.
Frailis, M.
Franceschi, E.
Frejsel, A.
Galeotta, S.
Galli, S.
Ganga, K.
Giard, M.
Giraud-Heraud, Y.
Gjerlow, E.
Gonzalez-Nuevo, J.
Gorski, K. M.
Gratton, S.
Gregorio, A.
Gruppuso, A.
Hansen, F. K.
Hanson, D.
Harrison, D. L.
Henrot-Versille, S.
Herranz, D.
Hildebrandt, S. R.
Hivon, E.
Hobson, M.
Holmes, W. A.
Hornstrup, A.
Hovest, W.
Huffenberger, K. M.
Hurier, G.
Jaffe, A. H.
Jaffe, T. R.
Juvela, M.
Keihanen, E.
Keskitalo, R.
Kiiveri, K.
Kisner, T. S.
Knoche, J.
Kunz, M.
Kurki-Suonio, H.
Lahteenmaki, A.
Lamarre, J. -M.
Lasenby, A.
Lattanzi, M.
Lawrence, C. R.
Leahy, J. P.
Leonardi, R.
Lesgourgues, J.
Levrier, F.
Liguori, M.
Lilje, P. B.
Linden-Vornle, M.
Lindholm, V.
Lopez-Caniego, M.
Lubin, P. M.
Macias-Perez, J. F.
Maggio, G.
Maino, D.
Mandolesi, N.
Mangilli, A.
Martin, P. G.
Martinez-Gonzalez, E.
Masi, S.
Matarrese, S.
Mazzotta, P.
McGehee, P.
Meinhold, P. R.
Melchiorri, A.
Mendes, L.
Mennella, A.
Migliaccio, M.
Mitra, S.
Montier, L.
Morgante, G.
Mortlock, D.
Moss, A.
Munshi, D.
Murphy, J. A.
Naselsky, P.
Nati, F.
Natoli, P.
Netterfield, C. B.
Norgaard-Nielsen, H. U.
Novikov, D.
Novikov, I.
Paci, F.
Pagano, L.
Paoletti, D.
Partridge, B.
Pasian, F.
Patanchon, G.
Pearson, T. J.
Perdereau, O.
Perotto, L.
Perrotta, F.
Pettorino, V.
Pierpaoli, E.
Pietrobon, D.
Pointecouteau, E.
Polenta, G.
Pratt, G. W.
Prezeau, G.
Prunet, S.
Puget, J. -L.
Rachen, J. P.
Rebolo, R.
Reinecke, M.
Remazeilles, M.
Renzi, A.
Rocha, G.
Rosset, C.
Rossetti, M.
Roudier, G.
Rubino-Martin, J. A.
Rusholme, B.
Sandri, M.
Santos, D.
Savelainen, M.
Scott, D.
Seiffert, M. D.
Shellard, E. P. S.
Spencer, L. D.
Stolyarov, V.
Stompor, R.
Sutton, D.
Suur-Uski, A. -S.
Sygnet, J. -F.
Tauber, J. A.
Terenzi, L.
Toffolatti, L.
Tomasi, M.
Tristram, M.
Tucci, M.
Tuovinen, J.
Valenziano, L.
Valiviita, J.
Van Tent, B.
Vassallo, T.
Vielva, P.
Villa, F.
Wade, L. A.
Wandelt, B. D.
Watson, R.
Wehus, I. K.
Yvon, D.
Zacchei, A.
Zonca, A.
CA Planck Collaboration
TI Planck 2015 results VI. LFI mapmaking
SO ASTRONOMY & ASTROPHYSICS
LA English
DT Article
DE cosmic background radiation; methods: data analysis
ID 30 GHZ DATA; CMB EXPERIMENTS; NOISE; MAPS; MADAM
AB This paper describes the mapmaking procedure applied to Planck Low Frequency Instrument (LFI) data. The mapmaking step takes as input the calibrated timelines and pointing information. The main products are sky maps of I, Q, and U Stokes components. For the first time, we present polarization maps at LFI frequencies. The mapmaking algorithm is based on a destriping technique, which is enhanced with a noise prior. The Galactic region is masked to reduce errors arising from bandpass mismatch and high signal gradients. We apply horn-uniform radiometer weights to reduce the effects of beam-shape mismatch. The algorithm is the same as used for the 2013 release, apart from small changes in parameter settings. We validate the procedure through simulations. Special emphasis is put on the control of systematics, which is particularly important for accurate polarization analysis. We also produce low-resolution versions of the maps and corresponding noise covariance matrices. These serve as input in later analysis steps and parameter estimation. The noise covariance matrices are validated through noise Monte Carlo simulations. The residual noise in the map products is characterized through analysis of half-ring maps, noise covariance matrices, and simulations.
C1 [Bucher, M.; Cardoso, J. -F.; Delabrouille, J.; Ganga, K.; Giraud-Heraud, Y.; Patanchon, G.; Remazeilles, M.; Rosset, C.; Roudier, G.; Stompor, R.] Univ Paris Diderot, Observ Paris, Sorbonne Paris Cite, APC,AstroParticule & Cosmol,CNRS,IN2P3,CEA,Irfu, 10 Rue Alice Domon & Leonie Duquet, F-75205 Paris 13, France.
[Lahteenmaki, A.] Aalto Univ, Metsahovi Radio Observ, POB 13000, Aalto 00076, Finland.
[Lahteenmaki, A.] Dept Radio Sci & Engn, POB 13000, Aalto 00076, Finland.
[Kunz, M.] African Inst Math Sci, 6-8 Melrose Rd, ZA-7945 Cape Town, South Africa.
[Natoli, P.; Polenta, G.] Agenzia Spaziale Italiana Sci Data Ctr, Via Politecn Snc, I-00133 Rome, Italy.
[Ashdown, M.; Curto, A.; Hobson, M.; Lasenby, A.; Stolyarov, V.] Univ Cambridge, Cavendish Lab, Astrophys Grp, JJ Thomson Ave, Cambridge CB3 0HE, England.
[Bond, J. R.; Hanson, D.; Martin, P. G.] Univ Toronto, CITA, 60 St George St, Toronto, ON M5S 3H8, Canada.
[Banday, A. J.; Bernard, J. -P.; Bielewic, P.; Forni, O.; Giard, M.; Jaffe, T. R.; Montier, L.; Pointecouteau, E.] IRAP, CNRS, 9 Av Colonel Roche,BP 44346, F-31028 Toulouse 4, France.
[Tuovinen, J.] Trinity Coll Dublin, CRANN, Dublin 2, Ireland.
[Crill, B. P.; Dore, O.; Hildebrandt, S. R.; Pearson, T. J.; Prezeau, G.; Rocha, G.; Seiffert, M. D.] CALTECH, Pasadena, CA 91125 USA.
[Fergusson, J.; Shellard, E. P. S.] Univ Cambridge, Ctr Theoret Cosmol, DAMTP, Wilberforce Rd, Cambridge CB3 0WA, England.
[Borrill, J.; Keskitalo, R.] Lawrence Berkeley Natl Lab, Computat Cosmol Ctr, Berkeley, CA 96153 USA.
[Rebolo, R.] CSIC, Plaza Murillo 2, E-28006 Madrid, Spain.
[Chamballu, A.; Yvon, D.] CEA Saclay, DSM Irfu SPP, F-91191 Gif Sur Yvette, France.
[Hornstrup, A.; Linden-Vornle, M.; Norgaard-Nielsen, H. U.] Tech Univ Denmark, Natl Space Inst, DTU Space, Elektrovej 327, DK-2800 Lyngby, Denmark.
[Kunz, M.; Tucci, M.] Univ Geneva, Dept Phys Theor, 24 Quai E Ansermet, CH-1211 Geneva 4, Switzerland.
[Toffolatti, L.] Univ Oviedo, Dept Fis, Calvo Sotelo S-N, Oviedo 33003, Spain.
[Netterfield, C. B.] Univ Toronto, Dept Astron & Astrophys, 50 St George St, Toronto, ON M55, Canada.
[Rachen, J. P.] Radboud Univ Nijmegen, Dept Astrophys IMAPP, POB 9010, NL-6500 GL Nijmegen, Netherlands.
[Scott, D.] Univ British Columbia, Dept Phys & Astron, 6224 Agr Rd, Vancouver, BC V6T 1Z4, Canada.
[Colombo, L. P. L.; Pierpaoli, E.] Univ Southern Calif, Dept Phys & Astron, Dana & David Dornsife Coll Letter Arts & Sci, Los Angeles, CA 90089 USA.
[Benoit-Levy, A.; Elsner, F.] UCL, Dept Phys & Astron, Mortimer St, London WC1E 6BT, England.
[Huffenberger, K. M.] Florida State Univ, Dept Phys, Keen Phys Bldg,77 Chieftan Way, Tallahassee, FL USA.
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[Nati, F.] Princeton Univ, Dept Phys, Princeton, NJ 08544 USA.
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[Renzi, A.] Univ Roma Tor Vergata, Dipartimento Matemat, Via Ric Sci 1, Rome, Italy.
[Christensen, P. R.] Niels Bohr Inst, Discovery Ctr, Blegdamsvej 17, DK-2100 Copenhagen, Denmark.
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[Pettorino, V.] HGSFP, Philosophenweg 16, D-69120 Heidelberg, Germany.
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[de Zotti, G.] Osserv Astron Padova, INAF, Vicolo Osservatorio 5, I-35141 Padua, Italy.
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[Mitra, S.] IUCAA, Post Bag 4,Pune Univ Campus, Pune 411007, Maharashtra, India.
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[Aghanim, N.; Aumont, J.; Chamballu, A.; Dole, H.; Douspis, M.; Hurier, G.; Kunz, M.; Mangilli, A.; Puget, J. -L.; Remazeilles, M.] Univ Paris Sud 11, Inst Astrophys Spatiale, CNRS, UMR8617, Batiment 121, F-91400 Orsay, France.
[Benabed, K.; Benoit-Levy, A.; Bouchet, F. R.; Cardoso, J. -F.; Colombi, S.; Ducout, A.; Elsner, F.; Galli, S.; Hivon, E.; Prunet, S.; Sygnet, J. -F.; Wandelt, B. D.] CNRS, Inst Astrophys Paris, UMR7095, 98 Bis Blvd Arago, F-75014 Paris, France.
[Efstathiou, G.; Gratton, S.; Harrison, D. L.; Migliaccio, M.; Sutton, D.] Univ Cambridge, Inst Astron, Madingley Rd, Cambridge CB3 0HA, England.
[Eriksen, H. K.; Gjerlow, E.; Hansen, F. K.; Lilje, P. B.] Univ Oslo, Inst Theoret Astrophys, N-0037 Oslo, Norway.
[Rebolo, R.; Rubino-Martin, J. A.] Inst Astrofis Canarias, C Via Lactea S-N, Tenerife 38205, Spain.
[Barreiro, R. B.; Bonavera, L.; Curto, A.; Diego, J. M.; Gonzalez-Nuevo, J.; Herranz, D.; Lopez-Caniego, M.; Martinez-Gonzalez, E.; Toffolatti, L.; Vielva, P.] Univ Cantabria, Inst Fis Cantabria, CSIC, Avda Castros S-N, E-39005 Santander, Spain.
[Bartolo, N.; Liguori, M.; Matarrese, S.] Ist Nazl Fis Nucl, Sez Padova, Via Marzolo 8, I-35131 Padua, Italy.
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[Ashdown, M.; Gratton, S.; Harrison, D. L.; Lasenby, A.; Migliaccio, M.; Stolyarov, V.; Sutton, D.] Kavli Inst Cosmol Cambridge, Madingley Rd, Cambridge CB3 0HA, England.
[Henrot-Versille, S.; Mangilli, A.; Perdereau, O.; Tristram, M.] Univ Paris 11, LAL, CNRS, IN2P3, F-91400 Orsay, France.
[Lesgourgues, J.] Univ Savoie, LAPTh, CNRS, BP 110, F-74941 Annecy Le Vieux, France.
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[Cardoso, J. -F.] CNRS, Lab Traitement & Commun Informat, UMR 5141, 46 Rue Barrault, F-75634 Paris 13, France.
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[Catalano, A.; Macias-Perez, J. F.; Perotto, L.; Santos, D.] Univ Grenoble Alpes, Lab Phys Subatom & Cosmol, CNRS, IN2P3, 53 Rue Martyrs, F-38026 Grenoble, France.
[Van Tent, B.] Univ Paris Sud 11, Phys Theor Lab, Batiment 210, F-91405 Orsay, France.
[Van Tent, B.] CNRS, Batiment 210, F-91405 Orsay, France.
[Kisner, T. S.] Lawrence Berkeley Natl Lab, Berkeley, CA 94720 USA.
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[Hanson, D.] McGill Univ, McGill Phys, Ernest Rutherford Phys Bldg,3600 Rue Univ, Montreal, PQ H3A 2T8, Canada.
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[Lesgourgues, J.] Ecole Polytech Fed Lausanne, SB ITP LPPC, CH-1015 Lausanne, Switzerland.
[Baccigalupi, C.; Bielewic, P.; Danese, L.; de Zotti, G.; Gonzalez-Nuevo, J.; Paci, F.; Perrotta, F.] SISSA, Astrophys Sect, Via Bonomea 265, I-34136 Trieste, Italy.
[Ade, P. A. R.; Munshi, D.; Spencer, L. D.] Cardiff Univ, Sch Phys & Astron, Queens Bldg, Cardiff CF24 3AA, S Glam, Wales.
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[Bouchet, F. R.] Sorbonne Univ, UPMC, Inst Astrophys Paris, UMR7095, 98 Bis Blvd Arago, F-75014 Paris, France.
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[Calabrese, E.] Univ Oxford, Subdept Astrophys, Keble Rd, Oxford OX1 3RH, England.
[Lesgourgues, J.] CERN, Div Theory, PH TH, CH-1211 Geneva 23, Switzerland.
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[Banday, A. J.; Bernard, J. -P.; Bielewic, P.; Forni, O.; Giard, M.; Jaffe, T. R.; Montier, L.; Pointecouteau, E.] Univ Toulouse, UPS OMP, IRAP, F-31028 Toulouse 4, France.
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RP Keihanen, E (reprint author), Univ Helsinki, Dept Phys, Gustaf Hallstromin Katu 2A, SF-00100 Helsinki, Finland.
EM elina.keihanen@helsinki.fi
RI Lahteenmaki, Anne/L-5987-2013; Barreiro, Rita Belen/N-5442-2014;
Mazzotta, Pasquale/B-1225-2016; bonavera, laura/E-9368-2017;
Gonzalez-Nuevo, Joaquin/I-3562-2014; Herranz, Diego/K-9143-2014;
Colombo, Loris/J-2415-2016;
OI Stolyarov, Vladislav/0000-0001-8151-828X; Barreiro, Rita
Belen/0000-0002-6139-4272; Mazzotta, Pasquale/0000-0002-5411-1748;
bonavera, laura/0000-0001-8039-3876; Gonzalez-Nuevo,
Joaquin/0000-0003-1354-6822; Herranz, Diego/0000-0003-4540-1417;
Colombo, Loris/0000-0003-4572-7732; Hivon, Eric/0000-0003-1880-2733;
Valiviita, Jussi/0000-0001-6225-3693; Kurki-Suonio,
Hannu/0000-0002-4618-3063; Zacchei, Andrea/0000-0003-0396-1192; Juvela,
Mika/0000-0002-5809-4834; Paoletti, Daniela/0000-0003-4761-6147;
TERENZI, LUCA/0000-0001-9915-6379; Toffolatti,
Luigi/0000-0003-2645-7386; Lilje, Per/0000-0003-4324-7794; Nati,
Federico/0000-0002-8307-5088; Pierpaoli, Elena/0000-0002-7957-8993
FU ESA; CNES (France); CNRS/INSU-IN2P3-INP (France); ASI (Italy); CNR
(Italy); INAF (Italy); NASA (USA); DoE (USA); STEC (UK); UKSA (UK); CSIC
(Spain); MINECO (Spain); J.A. (Spain); RES (Spain); Tekes (Finland); AoF
(Finland); CSC (Finland); DLR (Germany); MPG (Germany); CSA (Canada);
DTU Space (Denmark); SERISSO (Switzerland); RCN (Norway); SEI (Ireland);
FCT/MCTES (Portugal); ERC (EU); PRACE (EU); Office of Science of the US
Department of Energy [DE-AC02-05CH11231]; PRACE-3IP project [FP7
RI-312763]
FX The Planck Collaboration acknowledges the support of: ESA; CNES, and
CNRS/INSU-IN2P3-INP (France); ASI, CNR, and INAF (Italy); NASA and DoE
(USA); STEC and UKSA (UK); CSIC, MINECO, J.A., and RES (Spain); Tekes,
AoF, and CSC (Finland); DLR and MPG (Germany); CSA (Canada); DTU Space
(Denmark); SERISSO (Switzerland); RCN (Norway); SEI (Ireland); FCT/MCTES
(Portugal); ERC and PRACE (EU), A description of the Planck
Collaboration and a list of its members, indicating which technical or
scientific activities they have been involved in, can be found at
http//www.cosmos.eas.int/web/planck/planck-collaboration. Some of the
results of this research have been achieved using the PRACE-3IP project
(FP7 RI-312763) resource Sisu based in Finland at CSC. We thank CSC IT
Center for Science Ltd (Finland) for computational resources, This
research used resources of the National Energy Research Scientific
Computing Center, a DOE Office of Science User Facility supported by the
Office of Science of the US Department of Energy under Contract No.
DE-AC02-05CH11231, Iles work has made use of the Planck satellite
simulation package (Level-S), which is assembled by the Max Planck
Institute for Astrophysics Planck Analysis Centre (MPAC). Some of the
results in this paper have been derived urine the HEALPix package.
NR 43
TC 0
Z9 0
U1 0
U2 0
PU EDP SCIENCES S A
PI LES ULIS CEDEX A
PA 17, AVE DU HOGGAR, PA COURTABOEUF, BP 112, F-91944 LES ULIS CEDEX A,
FRANCE
SN 1432-0746
J9 ASTRON ASTROPHYS
JI Astron. Astrophys.
PD OCT
PY 2016
VL 594
AR A6
DI 10.1051/0004-6361/201525813
PG 23
WC Astronomy & Astrophysics
SC Astronomy & Astrophysics
GA DZ4MG
UT WOS:000385832200004
ER
PT J
AU Ade, PAR
Aghanim, N
Ashdown, M
Aumont, J
Baccigalupi, C
Banday, AJ
Barreiro, RB
Bartolo, N
Battaner, E
Benabed, K
Benoit, A
Benoit-Levy, A
Bernard, JP
Bersanelli, M
Bielewicz, P
Bock, JJ
Bonaldi, A
Bonavera, L
Bond, JR
Borrill, J
Bouchet, FR
Bucher, M
Burigana, C
Butler, RC
Calabrese, E
Cardoso, JF
Catalano, A
Chamballu, A
Christensen, PR
Colombi, S
Colombo, LPL
Crill, BP
Curto, A
Cuttaia, F
Danese, L
Davies, RD
Davis, RJ
de Bernardis, P
de Rosa, A
de Zotti, G
Delabrouille, J
Dickinson, C
Diego, JM
Dole, H
Donzelli, S
Dore, O
Douspis, M
Ducout, A
Dupac, X
Efstathiou, G
Elsner, F
Ensslin, TA
Eriksen, HK
Fergusson, J
Finelli, F
Forni, O
Frailis, M
Franceschi, E
Frejsel, A
Galeotta, S
Galli, S
Ganga, K
Giard, M
Giraud-Heraud, Y
Gjerlow, E
Gonzalez-Nuevo, J
Gorski, KM
Gratton, S
Gregorio, A
Gruppuso, A
Hansen, FK
Hanson, D
Harrison, DL
Henrot-Versille, S
Herranz, D
Hildebrandt, SR
Hivon, E
Hobson, M
Holmes, WA
Hornstrup, A
Hovest, W
Huffenberger, KM
Hurier, G
Jaffe, AH
Jaffe, TR
Juvela, M
Keihanen, E
Keskitalo, R
Kiiveri, K
Kisner, TS
Knoche, J
Kunz, M
Kurki-Suonio, H
Lahteenmaki, A
Lamarre, JM
Lasenby, A
Lattanzi, M
Lawrence, CR
Leahy, JP
Leonardi, R
Lesgourgues, J
Levrier, F
Liguori, M
Lilje, PB
Linden-Vornle, M
Lindholm, V
Lopez-Caniego, M
Lubin, PM
Macias-Perez, JF
Maggio, G
Maino, D
Mandolesi, N
Mangillin, A
Maris, M
Martin, PG
Martinez-Gonzalez, E
Masi, S
Matarrese, S
Mazzotta, P
McGehee, P
Meinhold, PR
Melchiorri, A
Mendes, L
Mennella, A
Migliaccio, M
Mitra, S
Montier, L
Morgante, G
Mortlock, D
Moss, A
Munshi, D
Murphy, JA
Naselsky, P
Nati, F
Natoli, P
Netterfield, CB
Norgaard-Nielsen, HU
Novikov, D
Novikov, I
Paci, F
Pagano, L
Paoletti, D
Partridge, B
Pasian, F
Patanchon, G
Pearson, TJ
Perdereau, O
Perotto, L
Perrotta, F
Pettorino, V
Piacentini, F
Pierpaoli, E
Pietrobon, D
Pointecouteau, E
Polenta, G
Pratt, GW
Prezeau, G
Prunet, S
Puget, JL
Rachen, JP
Rebolo, R
Reinecke, M
Remazeilles, M
Renzi, A
Rocha, G
Rosset, C
Rossetti, M
Roudier, G
Rubino-Martin, JA
Rusholme, B
Sandri, M
Santos, D
Savelainen, M
Scott, D
Seiffert, MD
Shellard, EPS
Spencer, LD
Stolyarov, V
Sutton, D
Suur-Uski, AS
Sygnet, JF
Tauber, JA
Terenzi, L
Toffolatti, L
Tomasi, M
Tristram, M
Tucci, M
Tuovinen, J
Umana, G
Valenziano, L
Valiviita, J
Van Tent, B
Vassallo, T
Vielva, P
Villa, F
Wade, LA
Wandelt, BD
Watson, R
Wehus, IK
Yvon, D
Zacchei, A
Zonca, A
AF Ade, P. A. R.
Aghanim, N.
Ashdown, M.
Aumont, J.
Baccigalupi, C.
Banday, A. J.
Barreiro, R. B.
Bartolo, N.
Battaner, E.
Benabed, K.
Benoit, A.
Benoit-Levy, A.
Bernard, J. -P.
Bersanelli, M.
Bielewicz, P.
Bock, J. J.
Bonaldi, A.
Bonavera, L.
Bond, J. R.
Borrill, J.
Bouchet, F. R.
Bucher, M.
Burigana, C.
Butler, R. C.
Calabrese, E.
Cardoso, J. -F.
Catalano, A.
Chamballu, A.
Christensen, P. R.
Colombi, S.
Colombo, L. P. L.
Crill, B. P.
Curto, A.
Cuttaia, F.
Danese, L.
Davies, R. D.
Davis, R. J.
de Bernardis, P.
de Rosa, A.
de Zotti, G.
Delabrouille, J.
Dickinson, C.
Diego, J. M.
Dole, H.
Donzelli, S.
Dore, O.
Douspis, M.
Ducout, A.
Dupac, X.
Efstathiou, G.
Elsner, F.
Ensslin, T. A.
Eriksen, H. K.
Fergusson, J.
Finelli, F.
Forni, O.
Frailis, M.
Franceschi, E.
Frejsel, A.
Galeotta, S.
Galli, S.
Ganga, K.
Giard, M.
Giraud-Heraud, Y.
Gjerlow, E.
Gonzalez-Nuevo, J.
Gorski, K. M.
Gratton, S.
Gregorio, A.
Gruppuso, A.
Hansen, F. K.
Hanson, D.
Harrison, D. L.
Henrot-Versille, S.
Herranz, D.
Hildebrandt, S. R.
Hivon, E.
Hobson, M.
Holmes, W. A.
Hornstrup, A.
Hovest, W.
Huffenberger, K. M.
Hurier, G.
Jaffe, A. H.
Jaffe, T. R.
Juvela, M.
Keihanen, E.
Keskitalo, R.
Kiiveri, K.
Kisner, T. S.
Knoche, J.
Kunz, M.
Kurki-Suonio, H.
Lahteenmaki, A.
Lamarre, J. -M.
Lasenby, A.
Lattanzi, M.
Lawrence, C. R.
Leahy, J. P.
Leonardi, R.
Lesgourgues, J.
Levrier, F.
Liguori, M.
Lilje, P. B.
Linden-Vornle, M.
Lindholm, V.
Lopez-Caniego, M.
Lubin, P. M.
Macias-Perez, J. F.
Maggio, G.
Maino, D.
Mandolesi, N.
Mangillin, A.
Maris, M.
Martin, P. G.
Martinez-Gonzalez, E.
Masi, S.
Matarrese, S.
Mazzotta, P.
McGehee, P.
Meinhold, P. R.
Melchiorri, A.
Mendes, L.
Mennella, A.
Migliaccio, M.
Mitra, S.
Montier, L.
Morgante, G.
Mortlock, D.
Moss, A.
Munshi, D.
Murphy, J. A.
Naselsky, P.
Nati, F.
Natoli, P.
Netterfield, C. B.
Norgaard-Nielsen, H. U.
Novikov, D.
Novikov, I.
Paci, F.
Pagano, L.
Paoletti, D.
Partridge, B.
Pasian, F.
Patanchon, G.
Pearson, T. J.
Perdereau, O.
Perotto, L.
Perrotta, F.
Pettorino, V.
Piacentini, F.
Pierpaoli, E.
Pietrobon, D.
Pointecouteau, E.
Polenta, G.
Pratt, G. W.
Prezeau, G.
Prunet, S.
Puget, J. -L.
Rachen, J. P.
Rebolo, R.
Reinecke, M.
Remazeilles, M.
Renzi, A.
Rocha, G.
Rosset, C.
Rossetti, M.
Roudier, G.
Rubino-Martin, J. A.
Rusholme, B.
Sandri, M.
Santos, D.
Savelainen, M.
Scott, D.
Seiffert, M. D.
Shellard, E. P. S.
Spencer, L. D.
Stolyarov, V.
Sutton, D.
Suur-Uski, A. -S.
Sygnet, J. -F.
Tauber, J. A.
Terenzi, L.
Toffolatti, L.
Tomasi, M.
Tristram, M.
Tucci, M.
Tuovinen, J.
Umana, G.
Valenziano, L.
Valiviita, J.
Van Tent, B.
Vassallo, T.
Vielva, P.
Villa, F.
Wade, L. A.
Wandelt, B. D.
Watson, R.
Wehus, I. K.
Yvon, D.
Zacchei, A.
Zonca, A.
CA Planck Collaboration
TI Planck 2015 results IV. Low Frequency Instrument beams and window
functions
SO ASTRONOMY & ASTROPHYSICS
LA English
DT Article
DE methods: data analysis; cosmic background radiation; telescopes
ID PRE-LAUNCH STATUS; LFI
AB This paper presents the characterization of the in-flight beams, the beam window functions, and the associated uncertainties for the Planck Low Frequency Instrument (LFI). The structure of the paper is similar to that presented in the 2013 Planck release; the main differences concern the beam normalization and the delivery of the window functions to be used for polarization analysis. The in-flight assessment of the LFI main beams relies on measurements performed during observations of Jupiter. By stacking data from seven Jupiter transits, the main beam profiles are measured down to -25 dB at 30 and 44 GHz, and down to -30 dB at 70 GHz. It has been confirmed that the agreement between the simulated beams and the measured beams is better than 1% at each LFI frequency band (within the 20 dB contour from the peak, the rms values are 0.1% at 30 and 70 GHz; 0.2% at 44 GHz). Simulated polarized beams are used for the computation of the effective beam window functions. The error budget for the window functions is estimated from both main beam and sidelobe contributions, and accounts for the radiometer band shapes. The total uncertainties in the effective beam window functions are 0.7% and 1% at 30 and 44 GHz, respectively (at l approximate to 600); and 0.5% at 70 GHz (at l approximate to 1000).
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[Battaner, E.] Univ Granada, Inst Carlos Fis Teor & Computac 1, Granada 18071, Spain.
[Gorski, K. M.] Univ Warsaw Observ, Aleje Ujazdowskie 4, PL-00478 Warsaw, Poland.
RP Sandri, M (reprint author), INAF IASF Bologna, Via Gobetti 101, I-40127 Bologna, Italy.
EM sandri@iasfbo.inaf.it
RI Lahteenmaki, Anne/L-5987-2013; Barreiro, Rita Belen/N-5442-2014;
Mazzotta, Pasquale/B-1225-2016; bonavera, laura/E-9368-2017;
Gonzalez-Nuevo, Joaquin/I-3562-2014; Herranz, Diego/K-9143-2014;
Colombo, Loris/J-2415-2016;
OI Juvela, Mika/0000-0002-5809-4834; Valiviita, Jussi/0000-0001-6225-3693;
Hurier, Guillaume/0000-0002-1215-0706; Hivon, Eric/0000-0003-1880-2733;
Toffolatti, Luigi/0000-0003-2645-7386; Paoletti,
Daniela/0000-0003-4761-6147; Nati, Federico/0000-0002-8307-5088;
Pierpaoli, Elena/0000-0002-7957-8993; TERENZI, LUCA/0000-0001-9915-6379;
Barreiro, Rita Belen/0000-0002-6139-4272; Mazzotta,
Pasquale/0000-0002-5411-1748; bonavera, laura/0000-0001-8039-3876;
Gonzalez-Nuevo, Joaquin/0000-0003-1354-6822; Herranz,
Diego/0000-0003-4540-1417; Colombo, Loris/0000-0003-4572-7732;
Kurki-Suonio, Hannu/0000-0002-4618-3063; Zacchei,
Andrea/0000-0003-0396-1192; Stolyarov, Vladislav/0000-0001-8151-828X
FU CNES; Italian Space Agency (ASI); INAF; Academy of Finland [253204,
256265, 257989, 283497]; PRACE-31P project [FP7 RI-312763]; Spanish
Ministerio de Ciencia e Innovacion through the Plan Nacional del Espacio
y Plan Nacional de Astronomia y Astrofisica; Space Agency of the German
Aerospace Center (DLR) [50OP0901]; Max Planck Society; National Energy
Research Scientific Computing Center; Office of Science of the US
Department of Energy [DE-AC02-05CH11231]; ESA; CNRS/INSU-IN2P3-INP
(France); ASI (Italy); CNR (Italy); INAF (Italy); NASA (USA); STFC (UK);
UKSA (UK); CSIC (Spain); MINECO (Spain); JA (Spain); RES (Spain); Tekes
(Finland); AoF (Finland); CSC (Finland); DLR (Germany); MPG (Germany);
CSA (Canada); DTU Space (Denmark); SER/SSO (Switzerland); RCN (Norway);
SFI (Ireland); FCT/MCTES (Portugal); ERC (EU); PRACE (EU); DoE (USA);
CNRS/INSU-IN2P3-INP; ASI
FX Planck is too large a project to allow full acknowledgement of all
contributions by individuals, institutions, industries, and funding
agencies. The main entities involved in the mission operations are as
follows. The European Space Agency (ESA) operates the satellite via its
Mission Operations Centre located at ESOC (Darmstadt, Germany) and
coordinates scientific operations via the Planck Science Office located
at ESAC (Madrid, Spain). Two Consortia, comprising around 50 scientific
institutes within Europe, the USA, and Canada, and funded by agencies
from the participating countries, developed the scientific instruments
LFI and HFI, and continue to operate them via Instrument Operations
Teams located in Trieste (Italy) and Orsay (France). The Consortia are
also responsible for scientific processing of the acquired data. The
Consortia are led by the Principal Investigators: J.L. Puget in France
for HFI (funded principally by CNES and CNRS/INSU-IN2P3-INP) and N.
Mandolesi in Italy for LFI (funded principally via ASI). NASA US Planck
Project, based at JPL and involving scientists at many US institutions,
contributes significantly to the efforts of these two Consortia. The
author list for this paper has been selected by the Planck Science Team,
and is composed of individuals from all of the above entities who have
made multi-year contributions to the development of the mission. It does
not pretend to be inclusive of all contributions. The Planck-LFI project
is developed by an International Consortium led by Italy and involving
Canada, Finland, Germany, Norway, Spain, Switzerland, UK, and USA. The
Italian contribution to Planck is supported by the Italian Space Agency
(ASI) and INAF. This work was supported by the Academy of Finland grants
253204, 256265, 257989, and 283497. We acknowledge that the results of
this research have been achieved using the PRACE-31P project (FP7
RI-312763) resource Sisu based in Finland at CSC. We thank CSC IT Center
for Science Ltd (Finland) for computational resources. We acknowledge
financial support provided by the Spanish Ministerio de Ciencia e
Innovacion through the Plan Nacional del Espacio y Plan Nacional de
Astronomia y Astrofisica. We acknowledge the Max Planck Institute for
Astrophysics Planck Analysis Centre (MPAC), funded by the Space Agency
of the German Aerospace Center (DLR) under grant 50OP0901 with resources
of the German Federal Ministry of Economics and Technology, and by the
Max Planck Society. This work has made use of the Planck satellite
simulation package (Level-S), which is assembled by the Max Planck
Institute for Astrophysics Planck Analysis Centre (MPAC). We acknowledge
financial support provided by the National Energy Research Scientific
Computing Center, which is supported by the Office of Science of the US
Department of Energy under Contract No. DE-AC02-05CH11231. Some of the
results in this paper have been derived using the HEALPix package. The
Planck Collaboration acknowledges the support of: ESA; CNES and
CNRS/INSU-IN2P3-INP (France); ASI, CNR, and INAF (Italy); NASA and DoE
(USA); STFC and UKSA (UK); CSIC, MINECO, JA, and RES (Spain); Tekes,
AoF, and CSC (Finland); DLR and MPG (Germany); CSA (Canada); DTU Space
(Denmark); SER/SSO (Switzerland); RCN (Norway); SFI (Ireland); FCT/MCTES
(Portugal); ERC and PRACE (EU). A description of the Planck
Collaboration and a list of its members, indicating which technical or
scientific activities they have been involved in, can be found at
http//maw.cosmos.esa.int/web/planck/planck-collaboration.
NR 49
TC 0
Z9 0
U1 0
U2 0
PU EDP SCIENCES S A
PI LES ULIS CEDEX A
PA 17, AVE DU HOGGAR, PA COURTABOEUF, BP 112, F-91944 LES ULIS CEDEX A,
FRANCE
SN 1432-0746
J9 ASTRON ASTROPHYS
JI Astron. Astrophys.
PD OCT
PY 2016
VL 594
AR A4
DI 10.1051/0004-6361/201525809
PG 22
WC Astronomy & Astrophysics
SC Astronomy & Astrophysics
GA DZ4MG
UT WOS:000385832200003
ER
PT J
AU Ade, PAR
Aghanim, N
Arnaud, M
Ashdown, M
Aumont, J
Baccigalupi, C
Banday, AJ
Barreiro, RB
Barrena, R
Bartlett, JG
Bartolo, N
Battaner, E
Battye, R
Benabed, K
Benoit, A
Benoit-Levy, A
Bernard, JP
Bersanelli, M
Bielewicz, P
Bikmaev, I
Bohringer, H
Bonaldi, A
Bonavera, L
Bond, JR
Borrill, J
Bouchet, FR
Bucher, M
Burenin, R
Burigana, C
Butler, RC
Calabrese, E
Cardoso, JF
Carvalho, P
Catalano, A
Challinor, A
Chamballu, A
Chary, RR
Chiang, HC
Chon, G
Christensen, PR
Clements, DL
Colombi, S
Colombo, LPL
Combet, C
Comis, B
Couchot, F
Coulais, A
Crill, BP
Curto, A
Cuttaia, F
Dahle, H
Danese, L
Davies, RD
Davis, RJ
de Bernardis, P
de Rosa, A
de Zotti, G
Delabrouille, J
Desert, FX
Dickinson, C
Diego, JM
Doag, K
Dole, H
Donzelli, S
Dore, O
Douspis, M
Ducout, A
Dupac, X
Efstathiou, G
Eisenhardt, PRM
Elsner, F
Ensslin, TA
Eriksen, HK
Falgarone, E
Fergusson, J
Feroz, F
Ferragamo, A
Finelli, F
Forni, O
Frailis, M
Fraisse, AA
Franceschi, E
Frejsel, A
Galeotta, S
Gai, S
Ganga, K
Genova-Santos, RT
Giard, M
Giraud-Heraud, Y
Gjerlow, E
Gonzalez-Nuevo, J
Gorski, KM
Grainge, KJB
Gratton, S
Gregorio, A
Gruppuso, A
Gudmundsson, JE
Hansen, FK
Hanson, D
Harrison, DL
Hempel, A
Henrot-Versille, S
Hernandez-Monteagudo, C
Herranz, D
Hildebrandt, SR
Hivon, E
Hobson, M
Holmes, WA
Hornstrup, A
Hovest, W
Huffenberger, KM
Hurier, G
Jaffe, AH
Jaffe, TR
Jin, T
Jones, WC
Juvela, M
Keihanen, E
Keskitalo, R
Khamitov, I
Kisner, TS
Kneissl, R
Knoche, J
Kunz, M
Kurki-Suonio, H
Lagache, G
Lamarre, JM
Lasenby, A
Lattanzi, M
Lawrence, CR
Leonardi, R
Lesgourgues, J
Levrier, F
Liguori, M
Lilje, PB
Linden-Vornle, M
Lopez-Caniego, M
Lubin, PM
Macias-Perez, JF
Maggio, G
Maino, D
Mak, DSY
Mandolesi, N
Mangilli, A
Martin, PG
Martinez-Gonzalez, E
Masi, S
Matarrese, S
Mazzotta, P
McGehee, P
Mei, S
Melchiorri, A
Melin, JB
Mendes, L
Mennella, A
Migliaccio, M
Mitra, S
Miville-Deschenes, MA
Moneti, A
Montier, L
Morgante, G
Mortlock, D
Mossl, A
Munshi, D
Murphy, JA
Naselsky, P
Nastasi, A
Nati, F
Natoli, P
Netterfield, CB
Norgaard-Nielsen, HU
Noviello, F
Novikov, D
Novikov, I
Olamaie, M
Oxborrow, CA
Paci, F
Pagano, L
Pajot, F
Paoletti, D
Pasian, F
Patanchon, G
Pearson, TJ
Perdereau, O
Perotto, L
Perron, YC
Perrotta, F
Pettorino, V
Piacentini, F
Piat, M
Pierpaoli, E
Pietrobon, D
Plaszczynski, S
Pointecouteau, E
Polenta, G
Pratt, GW
Prezeau, G
Prunet, S
Puget, JL
Rachen, JP
Reach, WT
Rebolo, R
Reinecke, M
Remazeilles, M
Renault, C
Renzi, A
Ristorcelli, I
Rocha, G
Rosset, C
Rossetti, M
Roudier, G
Rozo, E
Rubino-Martin, JA
Rumsey, C
Rusholme, B
Rykoff, ES
Sandri, M
Santos, D
Saunders, RDE
Savelainen, M
Savini, G
Schammel, MP
Scott, D
Seiffert, MD
Shellard, EPS
Shimwell, TW
Spencer, LD
Stanford, SA
Stern, D
Stolyarov, V
Stompor, R
Streblyanska, A
Sudiwala, R
Sunyaev, R
Sutton, D
Suur-Uski, AS
Sygnet, JF
Tauber, JA
Terenzi, L
Toffolatti, L
Tomasi, M
Tramonte, D
Tristram, M
Tucci, M
Tuovinen, J
Umana, G
Valenziano, L
Valiviita, J
Van Tent, B
Vielva, P
Villa, F
Wade, LA
Wandelt, BD
Wehus, IK
White, SDM
Wright, EL
Yvon, D
Zacchei, A
Zonca, A
AF Ade, P. A. R.
Aghanim, N.
Arnaud, M.
Ashdown, M.
Aumont, J.
Baccigalupi, C.
Banday, A. J.
Barreiro, R. B.
Barrena, R.
Bartlett, J. G.
Bartolo, N.
Battaner, E.
Battye, R.
Benabed, K.
Benoit, A.
Benoit-Levy, A.
Bernard, J. -P.
Bersanelli, M.
Bielewicz, P.
Bikmaev, I.
Boehringer, H.
Bonaldi, A.
Bonavera, L.
Bond, J. R.
Borrill, J.
Bouchet, F. R.
Bucher, M.
Burenin, R.
Burigana, C.
Butler, R. C.
Calabrese, E.
Cardoso, J. -F.
Carvalho, P.
Catalano, A.
Challinor, A.
Chamballu, A.
Chary, R. -R.
Chiang, H. C.
Chon, G.
Christensen, P. R.
Clements, D. L.
Colombi, S.
Colombo, L. P. L.
Combet, C.
Comis, B.
Couchot, F.
Coulais, A.
Crill, B. P.
Curto, A.
Cuttaia, F.
Dahle, H.
Danese, L.
Davies, R. D.
Davis, R. J.
de Bernardis, P.
de Rosa, A.
de Zotti, G.
Delabrouille, J.
Desert, F. -X.
Dickinson, C.
Diego, J. M.
Doag, K.
Dole, H.
Donzelli, S.
Dore, O.
Douspis, M.
Ducout, A.
Dupac, X.
Efstathiou, G.
Eisenhardt, P. R. M.
Elsner, F.
Ensslin, T. A.
Eriksen, H. K.
Falgarone, E.
Fergusson, J.
Feroz, F.
Ferragamo, A.
Finelli, F.
Forni, O.
Frailis, M.
Fraisse, A. A.
Franceschi, E.
Frejsel, A.
Galeotta, S.
Gai, S.
Ganga, K.
Genova-Santos, R. T.
Giard, M.
Giraud-Heraud, Y.
Gjerlow, E.
Gonzalez-Nuevo, J.
Gorski, K. M.
Grainge, K. J. B.
Gratton, S.
Gregorio, A.
Gruppuso, A.
Gudmundsson, J. E.
Hansen, F. K.
Hanson, D.
Harrison, D. L.
Hempel, A.
Henrot-Versille, S.
Hernandez-Monteagudo, C.
Herranz, D.
Hildebrandt, S. R.
Hivon, E.
Hobson, M.
Holmes, W. A.
Hornstrup, A.
Hovest, W.
Huffenberger, K. M.
Hurier, G.
Jaffe, A. H.
Jaffe, T. R.
Jin, T.
Jones, W. C.
Juvela, M.
Keihanen, E.
Keskitalo, R.
Khamitov, I.
Kisner, T. S.
Kneissl, R.
Knoche, J.
Kunz, M.
Kurki-Suonio, H.
Lagache, G.
Lamarre, J. -M.
Lasenby, A.
Lattanzi, M.
Lawrence, C. R.
Leonardi, R.
Lesgourgues, J.
Levrier, F.
Liguori, M.
Lilje, P. B.
Linden-Vornle, M.
Lopez-Caniego, M.
Lubin, P. M.
Macias-Perez, J. F.
Maggio, G.
Maino, D.
Mak, D. S. Y.
Mandolesi, N.
Mangilli, A.
Martin, P. G.
Martinez-Gonzalez, E.
Masi, S.
Matarrese, S.
Mazzotta, P.
McGehee, P.
Mei, S.
Melchiorri, A.
Melin, J. -B.
Mendes, L.
Mennella, A.
Migliaccio, M.
Mitra, S.
Miville-Deschenes, M. -A.
Moneti, A.
Montier, L.
Morgante, G.
Mortlock, D.
Mossl, A.
Munshi, D.
Murphy, J. A.
Naselsky, P.
Nastasi, A.
Nati, F.
Natoli, P.
Netterfield, C. B.
Norgaard-Nielsen, H. U.
Noviello, F.
Novikov, D.
Novikov, I.
Olamaie, M.
Oxborrow, C. A.
Paci, F.
Pagano, L.
Pajot, F.
Paoletti, D.
Pasian, F.
Patanchon, G.
Pearson, T. J.
Perdereau, O.
Perotto, L.
Perron, Y. C.
Perrotta, F.
Pettorino, V.
Piacentini, F.
Piat, M.
Pierpaoli, E.
Pietrobon, D.
Plaszczynski, S.
Pointecouteau, E.
Polenta, G.
Pratt, G. W.
Prezeau, G.
Prunet, S.
Puget, J. -L.
Rachen, J. P.
Reach, W. T.
Rebolo, R.
Reinecke, M.
Remazeilles, M.
Renault, C.
Renzi, A.
Ristorcelli, I.
Rocha, G.
Rosset, C.
Rossetti, M.
Roudier, G.
Rozo, E.
Rubino-Martin, J. A.
Rumsey, C.
Rusholme, B.
Rykoff, E. S.
Sandri, M.
Santos, D.
Saunders, R. D. E.
Savelainen, M.
Savini, G.
Schammel, M. P.
Scott, D.
Seiffert, M. D.
Shellard, E. P. S.
Shimwell, T. W.
Spencer, L. D.
Stanford, S. A.
Stern, D.
Stolyarov, V.
Stompor, R.
Streblyanska, A.
Sudiwala, R.
Sunyaev, R.
Sutton, D.
Suur-Uski, A. -S.
Sygnet, J. -F.
Tauber, J. A.
Terenzi, L.
Toffolatti, L.
Tomasi, M.
Tramonte, D.
Tristram, M.
Tucci, M.
Tuovinen, J.
Umana, G.
Valenziano, L.
Valiviita, J.
Van Tent, B.
Vielva, P.
Villa, F.
Wade, L. A.
Wandelt, B. D.
Wehus, I. K.
White, S. D. M.
Wright, E. L.
Yvon, D.
Zacchei, A.
Zonca, A.
CA Planck Collaboration
TI Planck 2015 results XXVII. The second Planck catalogue of
Sunyaev-Zeldovich sources
SO ASTRONOMY & ASTROPHYSICS
LA English
DT Article
DE cosmology: observations; galaxies: clusters: general; catalogs
ID GALAXY CLUSTER SURVEY; DIGITAL SKY SURVEY; X-RAY-PROPERTIES; DISCRETE
OBJECT DETECTION; INFRARED-SURVEY-EXPLORER; ASTRONOMICAL DATA SETS; FAST
BAYESIAN-APPROACH; POLE TELESCOPE SURVEY; SCALING RELATIONS;
COSMOLOGICAL CONSTRAINTS
AB We present the all-sky Planck catalogue of Sunyaev-Zeldovich (SZ) sources detected from the 29 month full-mission data. The catalogue (PSZ2) is the largest SZ-selected sample of galaxy clusters yet produced and the deepest systematic all-sky survey of galaxy clusters. It contains 1653 detections, of which 1203 are confirmed clusters with identified counterparts in external data sets, and is the first SZ-selected cluster survey containing > 10(3) confirmed clusters. We present a detailed analysis of the survey selection function in terms of its completeness and statistical reliability, placing a lower limit of 83% on the purity. Using simulations, we find that the estimates of the SZ strength parameter Y-5R500 are robust to pressure-profile variation and beam systematics, but accurate conversion to Y-500 requires the use of prior information on the cluster extent. We describe the multi-wavelength search for counterparts in ancillary data, which makes use of radio, microwave, infra-red, optical, and X-ray data sets, and which places emphasis on the robustness of the counterpart match. We discuss the physical properties of the new sample and identify a population of low-redshift X-ray under-luminous clusters revealed by SZ selection. These objects appear in optical and SZ surveys with consistent properties for their mass, but are almost absent from ROSAT X-ray selected samples.
C1 [Bartlett, J. G.; Bucher, M.; Cardoso, J. -F.; Delabrouille, J.; Ganga, K.; Giraud-Heraud, Y.; Patanchon, G.; Piat, M.; Remazeilles, M.; Rosset, C.; Roudier, G.; Stompor, R.] Univ Paris Diderot, Sorbonne Paris Cite, CEA Irfu,Observ Paris, APC,AstroParticule & Cosmol,CNRS IN2P3, 10 Rue Alice Domon & Leonie Duquet, F-75205 Paris 13, France.
[Bikmaev, I.] Acad Sci Tatarstan, Bauman Str 20, Kazan 420111, Russia.
[Kunz, M.] African Inst Math Sci, 6-8 Melrose Rd, Cape Town, South Africa.
[Natoli, P.; Polenta, G.] Agenzia Spaziale Italiana Sci Data Ctr, Via Politecn Snc, I-00133 Rome, Italy.
[Lagache, G.] Aix Marseille Univ, CNRS, LAM, UMR 7326, F-13388 Marseille, France.
[Ashdown, M.; Curto, A.; Feroz, F.; Grainge, K. J. B.; Hobson, M.; Jin, T.; Lasenby, A.; Olamaie, M.; Perron, Y. C.; Rumsey, C.; Saunders, R. D. E.; Schammel, M. P.; Shimwell, T. W.; Stolyarov, V.] Univ Cambridge, Cavendish Lab, Astrophys Grp, JJ Thomson Ave, Cambridge CB3 0HE, England.
[Chiang, H. C.] Univ KwaZulu Natal, Sch Math Stat & Comp Sci, Astrophys & Cosmol Res Unit, Westville Campus,Private Bag X54001, ZA-4000 Durban, South Africa.
[Kneissl, R.] ALMA Santiago Cent Off, Atacama Large Millimeter Submillimeter Array, Alonso de Cordova 3107,Casilla 7630355, Santiago, Chile.
[Bond, J. R.; Hanson, D.; Martin, P. G.; Miville-Deschenes, M. -A.] Univ Toronto, CITA, 60 St George St, Toronto, ON M5S 3H8, Canada.
[Banday, A. J.; Bernard, J. -P.; Bielewicz, P.; Forni, O.; Giard, M.; Jaffe, T. R.; Montier, L.; Pointecouteau, E.; Ristorcelli, I.] IRAP, CNRS, 9 Av Colonel Roche,BP 44346, F-31028 Toulouse 4, France.
[Tuovinen, J.] Trinity Coll Dublin, CRANN, Dublin 2, Ireland.
[Crill, B. P.; Dore, O.; Hildebrandt, S. R.; Mei, S.; Pearson, T. J.; Prezeau, G.; Rocha, G.; Seiffert, M. D.] CALTECH, Pasadena, CA 91125 USA.
[Challinor, A.; Fergusson, J.; Shellard, E. P. S.] Univ Cambridge, Ctr Theoret Cosmol, DAMTP, Wilberforce Rd, Cambridge CB3 0WA, England.
[Hernandez-Monteagudo, C.] CEFCA, Plaza San Juan 1,Planta 2, Teruel 44001, Spain.
[Borrill, J.; Keskitalo, R.] Lawrence Berkeley Natl Lab, Computat Cosmol Ctr, Berkeley, CA USA.
[Rebolo, R.] CSIC, E-28049 Madrid, Spain.
[Chamballu, A.; Melin, J. -B.; Yvon, D.] CEA Saclay, DSM Irfu SPP, F-91191 Gif Sur Yvette, France.
[Hornstrup, A.; Linden-Vornle, M.; Norgaard-Nielsen, H. U.; Oxborrow, C. A.] Tech Univ Denmark, Natl Space Inst, DTU Space, Elektrovej 327, DK-2800 Lyngby, Denmark.
[Kunz, M.; Tucci, M.] Univ Geneva, Dept Phys Theor, 24 Quai E Ansermet, CH-1211 Geneva 4, Switzerland.
[Ferragamo, A.; Streblyanska, A.] Univ La Laguna, Dept Astrofis, E-38206 Tenerife, Spain.
[Toffolatti, L.] Univ Oviedo, Dept Fis, Avda Calvo Sotelo S-N, Oviedo 33007, Spain.
[Netterfield, C. B.] Univ Toronto, Dept Astron & Astrophys, 50 St George St, Toronto, ON 38100, Canada.
[Bikmaev, I.; Khamitov, I.] Kazan Fed Univ, Dept Astron & Geodesy, Kremlevskaya Str 18, Kazan 420008, Russia.
[Rachen, J. P.] Radboud Univ Nijmegen, Dept Astrophys IMAPP, POB 9010, NL-6500 GL Nijmegen, Netherlands.
[Scott, D.] Univ British Columbia, Dept Phys & Astron, 6224 Agr Rd, Vancouver, BC, Canada.
[Colombo, L. P. L.; Mak, D. S. Y.; Pierpaoli, E.] Univ Southern Calif, Dana & David Dornsife Coll Letter Arts & Sci, Dept Phys & Astron, Los Angeles, CA 90089 USA.
[Benoit-Levy, A.; Elsner, F.] UCL, Dept Phys & Astron, London WC1E 6BT, England.
[Huffenberger, K. M.] Florida State Univ, Dept Phys, Keen Phys Bldg,77 Chieftan Way, Tallahassee, FL 32306 USA.
[Juvela, M.; Keihanen, E.; Kurki-Suonio, H.; Savelainen, M.; Suur-Uski, A. -S.; Valiviita, J.] Univ Helsinki, Dept Phys, Gustaf Hallstromin Katu 2A, Helsinki 00560, Finland.
[Chiang, H. C.; Gudmundsson, J. E.; Jones, W. C.; Nati, F.] Princeton Univ, Dept Phys, Princeton, NJ 08544 USA.
[Rozo, E.] Univ Arizona, Dept Phys, 1118 E 4th St, Tucson, AZ 85721 USA.
[Stanford, S. A.] Univ Calif Davis, Dept Phys, One Shields Ave, Davis, CA USA.
[Lubin, P. M.; Zonca, A.] Univ Calif Santa Barbara, Dept Phys, Santa Barbara, CA 95616 USA.
[Wandelt, B. D.] Univ Illinois, Dept Phys, 1110 West Green St, Urbana, CA 93106 USA.
[Bartolo, N.; Liguori, M.; Matarrese, S.] Univ Padua, Dipartimento Fis & Astron G Galilei, Via Marzolo 8, I-35131 Padua, Italy.
[Burigana, C.; Lattanzi, M.; Mandolesi, N.; Natoli, P.] Univ Ferrara, Dipartimento Fis & Sci Terra, Via Saragat 1, I-44122 Ferrara, Italy.
[de Bernardis, P.; Masi, S.; Melchiorri, A.; Pagano, L.; Piacentini, F.] Univ Roma La Sapienza, Dipartimento Fis, Ple A Moro 2, I-00133 Rome, Italy.
[Bersanelli, M.; Maino, D.; Mennella, A.; Rossetti, M.; Tomasi, M.] Univ Milan, Dipartimento Fis, Via Celoria 16, I-20133 Milan, Italy.
[Gregorio, A.] Univ Trieste, Dipartimento Fis, Via A Valerio 2, I-34127 Trieste, Italy.
[Mazzotta, P.] Univ Roma Tor Vergata, Dipartimento Fis, Via Ric Sci 1, I-00133 Rome, Italy.
[Renzi, A.] Univ Roma Tor Vergata, Dipartimento Matemat, Via Ric Sci 1, I-00133 Rome, Italy.
[Christensen, P. R.; Naselsky, P.] Niels Bohr Inst, Discovery Ctr, Blegdamsvej 17, DK-1165 Copenhagen, Denmark.
[Barrena, R.; Genova-Santos, R. T.; Hempel, A.; Rebolo, R.; Rubino-Martin, J. A.; Tramonte, D.] ULL, Dept Astrofis, Tenerife 38206, Spain.
[Kneissl, R.] European Southern Observ, ESO Vitacura, Alonso de Cordova 3107,Casilla 19001, Santiago, Chile.
[Dupac, X.; Leonardi, R.; Lopez-Caniego, M.; Mendes, L.] European Space Agcy, ESAC, Planck Sci Off, Camino Bajo Castillo S-N, Madrid 28691, Spain.
[Tauber, J. A.] European Space Agcy, Estec, Keplerlaan 1, NL-2201 AZ Noordwijk, Netherlands.
[Terenzi, L.] Univ E Campus, Fac Ingn, Via Isimbardi 10, I-22060 Novedrate, CO, Italy.
[Mei, S.] Observ Paris, GEPI, Sect Meudon, 5 Pl J Janssen, F-92195 Meudon, France.
[Matarrese, S.] Ist Nazl Fis Nucl, Gran Sasso Sci Inst, Viale F Crispi 7, I-67100 Laquila, Italy.
[Pettorino, V.] HGSFP, Philosophenweg 16, D-69120 Heidelberg, Germany.
[Pettorino, V.] Heidelberg Univ, Dept Theoret Phys, Philosophenweg 16, D-69120 Heidelberg, Germany.
[Kurki-Suonio, H.; Savelainen, M.; Suur-Uski, A. -S.; Valiviita, J.] Univ Helsinki, Helsinki Inst Phys, Gustaf Hallstromin Katu 2, 00560 Helsinki, Finland.
[Umana, G.] INAF Osservatorio Astrofis Catania, Via S Sofia 78, Catania, Italy.
[de Zotti, G.] INAF Osservatorio Astron Padova, Vicolo Osservatorio 5, I-35131 Padua, Italy.
[Polenta, G.] INAF Osservatorio Astron Roma, Via Frascati 33, I-00040 Monte Porzio Catone, Italy.
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[Burigana, C.; Butler, R. C.; Cuttaia, F.; de Rosa, A.; Finelli, F.; Franceschi, E.; Gruppuso, A.; Mandolesi, N.; Morgante, G.; Natoli, P.; Paoletti, D.; Sandri, M.; Terenzi, L.; Toffolatti, L.; Valenziano, L.; Villa, F.] INAF IASF Bologna, Via Gobetti 101, I-40127 Bologna, Italy.
[Bersanelli, M.; Donzelli, S.; Maino, D.; Mennella, A.; Rossetti, M.; Tomasi, M.] INAF IASF Milano, Via E Bassini 15, I-20133 Milan, Italy.
[Burigana, C.; Finelli, F.; Paoletti, D.] Ist Nazl Fis Nucl, Sez Bologna, Via Irnerio 46, I-40126 Bologna, Italy.
[Melchiorri, A.; Pagano, L.] Univ Roma Sapienza, Ist Nazl Fis Nucl, Sez Roma 1, Piazzale Aldo Moro 2, I-00185 Rome, Italy.
[Renzi, A.] Univ Roma Tor Vergata, Ist Nazl Fis Nucl, Sez Roma 2, Via Ric Sci, Rome 1, Italy.
[Gregorio, A.] INFN Natl Inst Nucl Phys, Via Valerio 2, I-34127 Trieste, Italy.
[Desert, F. -X.] IPAG, F-38000 Grenoble, France.
[Desert, F. -X.] Univ Grenoble Alpes, IPAG, Inst Planetol & Astrophys Grenoble, F-38000 Grenoble, France.
[Desert, F. -X.] CNRS, IPAG, F-38000 Grenoble, France.
[Mitra, S.] IUCAA, Post Bag 4,Pune Univ Campus, Pune 411007, Maharashtra, India.
[Clements, D. L.; Ducout, A.; Jaffe, A. H.; Mortlock, D.] Imperial Coll London, Astrophys Grp, Blackett Lab, Prince Consort Rd, London SW7 2AZ, England.
[Chary, R. -R.; McGehee, P.; Pearson, T. J.; Rusholme, B.] CALTECH, Infrared Proc & Anal Ctr, Pasadena, CA 91125 USA.
[Benoit, A.] Univ Joseph Fourier Grenoble I, CNRS, Inst Neel, 25 Rue Martyrs, F-38042 Grenoble, France.
[Dole, H.] Inst Univ France, 103 Bd St Michel, F-75005 Paris, France.
[Aghanim, N.; Aumont, J.; Chamballu, A.; Dole, H.; Douspis, M.; Hurier, G.; Kunz, M.; Lagache, G.; Mangilli, A.; Miville-Deschenes, M. -A.; Nastasi, A.; Pajot, F.; Puget, J. -L.; Remazeilles, M.] Univ Paris Sud 11, CNRS, Inst Astrophys Spatiale, UMR8617, Batiment 121, F-91898 Orsay, France.
[Benabed, K.; Benoit-Levy, A.; Bouchet, F. R.; Cardoso, J. -F.; Colombi, S.; Ducout, A.; Elsner, F.; Gai, S.; Hivon, E.; Moneti, A.; Prunet, S.; Sygnet, J. -F.; Wandelt, B. D.] CNRS, Inst Astrophys Paris, UMR7095, 98 Bis Blvd Arago, F-75014 Paris, France.
[Carvalho, P.; Challinor, A.; Efstathiou, G.; Gratton, S.; Harrison, D. L.; Migliaccio, M.; Sutton, D.] Univ Cambridge, Inst Astron, Madingley Rd, Cambridge CB3 0HA, England.
[Barrena, R.; Dahle, H.; Eriksen, H. K.; Gjerlow, E.; Hansen, F. K.; Lilje, P. B.] Univ Oslo, Inst Theoret Astrophys, N-0371 Oslo, Norway.
[Genova-Santos, R. T.; Hempel, A.; Rebolo, R.; Rubino-Martin, J. A.; Tramonte, D.] Inst Astrofis Canarias, C Via Lactea S-N, Tenerife 38205, Spain.
[Ferragamo, A.; Streblyanska, A.] Inst Astrofis Canarias, Tenerife 38200, Spain.
[Barreiro, R. B.; Bonavera, L.; Curto, A.; Diego, J. M.; Gonzalez-Nuevo, J.; Herranz, D.; Lopez-Caniego, M.; Martinez-Gonzalez, E.; Toffolatti, L.; Vielva, P.] Univ Cantabria, CSIC, Inst Fis Cantabria, Avda Castros S-N, E-39005 Santander, Spain.
[Schammel, M. P.] Ist Nazl Astrofis, Osservatorio Astron Roma, Via Frascati 33, I-00040 Monte Porzio Catone, RM, Italy.
[Bartolo, N.; Liguori, M.; Matarrese, S.] Ist Nazl Fis Nucl, Sez Padova, Via Marzolo 8, I-35131 Padua, Italy.
[Bartlett, J. G.; Colombo, L. P. L.; Crill, B. P.; Dore, O.; Eisenhardt, P. R. M.; Gorski, K. M.; Hanson, D.; Hildebrandt, S. R.; Holmes, W. A.; Lawrence, C. R.; Mitra, S.; Pietrobon, D.; Prezeau, G.; Rocha, G.; Roudier, G.; Seiffert, M. D.; Stern, D.; Wade, L. A.; Wehus, I. K.] CALTECH, Jet Prop Lab, 4800 Oak Grove Dr, Pasadena, CA 91125 USA.
[Battye, R.; Bonaldi, A.; Davies, R. D.; Davis, R. J.; Dickinson, C.; Noviello, F.; Remazeilles, M.] Univ Manchester, Sch Phys & Astron, Jodrell Bank Ctr Astrophys, Alan Turing Bldg,Oxford Rd, Manchester M13 9PL, Lancs, England.
[Ashdown, M.; Carvalho, P.; Challinor, A.; Grainge, K. J. B.; Gratton, S.; Harrison, D. L.; Lasenby, A.; Migliaccio, M.; Stolyarov, V.; Sutton, D.] Kavli Inst Cosmol Cambridge, Madingley Rd, Cambridge CB3 0HA, England.
[Couchot, F.; Henrot-Versille, S.; Mangilli, A.; Perdereau, O.; Plaszczynski, S.; Tristram, M.] Univ Paris 11, CNRS IN2P3, LAL, Orsay, France.
[Lesgourgues, J.] Univ Savoie, LAPTh, CNRS, BP 110, F-74941 Annecy Le Vieux, France.
[Catalano, A.; Coulais, A.; Falgarone, E.; Lamarre, J. -M.; Levrier, F.; Roudier, G.] CNRS, Observ Paris, LERMA, 61 Ave Observ, F-75000 Paris, France.
[Arnaud, M.; Chamballu, A.; Pratt, G. W.] Univ Paris Diderot, CEA Saclay, CNRS, Lab AIM,IRFU,Serv Astrophys,CEA,DSM, Bat 709, F-91191 Gif Sur Yvette, France.
[Cardoso, J. -F.] CNRS, UMR 5141, Lab Traitement & Commun Informat, 46 Rue Barrault, F-75634 Paris 13, France.
[Cardoso, J. -F.] Telecom ParisTech, 46 Rue Barrault, F-75634 Paris 13, France.
[Catalano, A.; Combet, C.; Comis, B.; Macias-Perez, J. F.; Perotto, L.; Renault, C.; Santos, D.] Univ Grenoble Alpes, CNRS IN2P3, Lab Phys Subat & Cosmol, 53 Rue Martyrs, F-38026 Grenoble, France.
[Van Tent, B.] Univ Paris Sud 11, Lab Phys Theor, Batiment 210, F-91405 Orsay, France.
[Van Tent, B.] CNRS, Batiment 210, F-91405 Orsay, France.
[Kisner, T. S.] Lawrence Berkeley Natl Lab, Berkeley, CA 94720 USA.
[Novikov, D.; Novikov, I.] Russian Acad Sci, Ctr Astro Space, Lebedev Phys Inst, 84-32 Profsoyuznaya St,GSP-7, Moscow 117997, Russia.
[Doag, K.; Ensslin, T. A.; Hernandez-Monteagudo, C.; Hovest, W.; Knoche, J.; Rachen, J. P.; Reinecke, M.; Sunyaev, R.; White, S. D. M.] Max Planck Inst Astrophys, Karl Schwarzschild Str 1, D-85741 Garching, Germany.
[Boehringer, H.; Chon, G.] Max Planck Inst Extraterr Phys, Giessenbachstr, D-85748 Garching, Germany.
[Hanson, D.] McGill Univ, McGill Phys, Ernest Rutherford Phys Bldg,3600 Rue Univ, Montreal, PQ H3A 2T8, Canada.
[Burenin, R.] Moscow Inst Phys & Technol, Inst Sky Per 9, Dolgoprudnyi 141700, Russia.
[Murphy, J. A.] Natl Univ Ireland, Dept Expt Phys, Maynooth, Kildare, Ireland.
[Christensen, P. R.; Frejsel, A.; Naselsky, P.; Novikov, I.] Niels Bohr Inst, Blegdamsvej 17, DK-1165 Copenhagen, Denmark.
[Savini, G.] UCL, Opt Sci Lab, Gower St, London, England.
[Lesgourgues, J.] Ecole Polytech Fed Lausanne, SB ITP LPPC, CH-1015 Lausanne, Switzerland.
[Baccigalupi, C.; Bielewicz, P.; Danese, L.; de Zotti, G.; Gonzalez-Nuevo, J.; Paci, F.; Perrotta, F.] SISSA, Astrophys Sect, Via Bonomea 265, I-34136 Trieste, Italy.
[Rykoff, E. S.] SLAC Natl Accelerator Lab, Menlo Pk, CA 94025 USA.
[Ade, P. A. R.; Munshi, D.; Spencer, L. D.; Sudiwala, R.] Cardiff Univ, Sch Phys & Astron, Queens Bldg, Cardiff CF24 3AA, S Glam, Wales.
[Mossl, A.] Univ Nottingham, Sch Phys & Astron, Nottingham NG7 2RD, England.
[Bouchet, F. R.] Sorbonne Univ UPMC, Inst Astrophys Paris, UMR7095, 98 Bis Blvd Arago, F-75014 Paris, France.
[Burenin, R.; Sunyaev, R.] Russian Acad Sci, Space Res Inst IKI, Profsoyuznaya Str 84-32, Moscow 117997, Russia.
[Borrill, J.] Univ Calif Berkeley, Space Sci Lab, Berkeley, CA 94720 USA.
[Stolyarov, V.] Russian Acad Sci, Special Astrophys Observ, Karachai Cherkessian Rep 369167, Zelenchukskiy R, Russia.
[Shimwell, T. W.] Sterrewacht Leiden, POB 9513, NL-2300 RA Leiden, Netherlands.
[Calabrese, E.] Univ Oxford, Subdept Astrophys, Keble Rd, Oxford OX1 3RH, England.
[Khamitov, I.] TUBITAK Natl Observ, Akdeniz Univ Campus, TR-07058 Antalya, Turkey.
[Lesgourgues, J.] CERN, Div Theory, PH TH, CH-1211 Geneva 23, Switzerland.
[Wright, E. L.] Univ Calif Los Angeles, Astron, POB 951547, Los Angeles, CA 90095 USA.
[Benabed, K.; Benoit-Levy, A.; Colombi, S.; Elsner, F.; Hivon, E.; Prunet, S.; Wandelt, B. D.] UPMC Univ Paris 06, UMR7095, 98 Bis Blvd Arago, F-75014 Paris, France.
[Hempel, A.] Univ Andres Bello, Fac Ciencias Exactas, Dept Ciencias Fis, Santiago 8370134, Chile.
[Mei, S.] Univ Denis Diderot Paris 7, F-75205 Paris 13, France.
[Banday, A. J.; Bernard, J. -P.; Bielewicz, P.; Forni, O.; Giard, M.; Jaffe, T. R.; Montier, L.; Pointecouteau, E.; Ristorcelli, I.] Univ Toulouse, UPS OMP, IRAP, F-31028 Toulouse 4, France.
[Reach, W. T.] Univ Space Res Assoc, Stratospher Observ Infrared Astron, MS 232-11, Moffett Field, CA 94035 USA.
[Doag, K.] Ludwig Maximilian Univ Munich, Univ Observ, Scheinerstr 1, D-81679 Munich, Germany.
[Battaner, E.] Univ Granada, Dept Fis Teor & Cosmos, Fac Ciencias, E-18071 Granada, Spain.
[Battaner, E.] Univ Granada, Inst Carlos 1 Fis Teor & Computac, E-18071 Granada, Spain.
[Gorski, K. M.] Univ Warsaw Observ, Aleje Ujazdowskie 4, PL-00478 Warsaw, Poland.
RP Sutton, D (reprint author), Univ Cambridge, Inst Astron, Madingley Rd, Cambridge CB3 0HA, England.; Sutton, D (reprint author), Kavli Inst Cosmol Cambridge, Madingley Rd, Cambridge CB3 0HA, England.
EM sutton@ast.cam.ac.uk
RI Barreiro, Rita Belen/N-5442-2014; Mazzotta, Pasquale/B-1225-2016;
bonavera, laura/E-9368-2017; Gonzalez-Nuevo, Joaquin/I-3562-2014;
Herranz, Diego/K-9143-2014; Colombo, Loris/J-2415-2016;
OI Hurier, Guillaume/0000-0002-1215-0706; Barreiro, Rita
Belen/0000-0002-6139-4272; Mazzotta, Pasquale/0000-0002-5411-1748;
bonavera, laura/0000-0001-8039-3876; Gonzalez-Nuevo,
Joaquin/0000-0003-1354-6822; Herranz, Diego/0000-0003-4540-1417;
Colombo, Loris/0000-0003-4572-7732; TERENZI, LUCA/0000-0001-9915-6379;
Stolyarov, Vladislav/0000-0001-8151-828X; Reach,
William/0000-0001-8362-4094; Valiviita, Jussi/0000-0001-6225-3693;
Kurki-Suonio, Hannu/0000-0002-4618-3063; Zacchei,
Andrea/0000-0003-0396-1192; Toffolatti, Luigi/0000-0003-2645-7386;
Lilje, Per/0000-0003-4324-7794; Paoletti, Daniela/0000-0003-4761-6147;
Nati, Federico/0000-0002-8307-5088; Savini, Giorgio/0000-0003-4449-9416;
Pierpaoli, Elena/0000-0002-7957-8993; Juvela, Mika/0000-0002-5809-4834
FU ESA; CNES (France); CNRS/INSU-IN2P3-INP (France); ASI (Italy); CNR
(Italy); INAF (Italy); NASA (USA); DoE (USA); STFC (UK); UKSA (UK); CSIC
(Spain); MINECO (Spain); JA (Spain); RES (Spain); Tekes (Finland); AoF
(Finland); CSC (Finland); DLR (Germany); MPG (Germany); CSA (Canada);
DTU Space (Denmark); SER/SSO (Switzerland); RCN (Norway); SFI (Ireland);
FCT/MCTES (Portugal); ERC (EU); PRACE (EU); Higher Education Funding
Council for England; Science and Technology Facilities Council; Alfred
P. Sloan Foundation; National Science Foundation; US Department of
Energy Office of Science
FX The Planck Collaboration acknowledges the support of: ESA; CNES and
CNRS/INSU-IN2P3-INP (France); ASI, CNR, and INAF (Italy); NASA and DoE
(USA); STFC and UKSA (UK); CSIC, MINECO, JA, and RES (Spain); Tekes,
AoF, and CSC (Finland); DLR and MPG (Germany); CSA (Canada); DTU Space
(Denmark); SER/SSO (Switzerland); RCN (Norway); SFI (Ireland); FCT/MCTES
(Portugal); ERC and PRACE (EU). A description of the Planck
Collaboration and a list of its members, indicating which technical or
scientific activities they have been involved in, can be found at
http://www.cosmos.esa.int/web/planck/plancks-collaboration. We thank Ian
McCarthy for providing images and profiles of simulated clusters from
cosmo-OWLS. This research has made use of the NASA/IPAC Extragalactic
Database (NED), which is operated by the Jet Propulsion Laboratory,
California Institute of Technology, under contract with the National
Aeronautics and Space Administration, and the SIMBAD database, operated
at CDS, Strasbourg, France This research made use of data retrieved from
SDSS-III. Funding for SDSS-III has been provided by the Alfred P. Sloan
Foundation, the Participating Institutions, the National Science
Foundation, and the US Department of Energy Office of Science; the
SDSS-III web site is http://www.sdss3.ore/. This research has made use
of data processed by the Centre d'Analyse de Donnees Etendues
(http://www.cade.irap.omp.eu/) and has made use of the HEALPix
pixelization software (http://healpix.sourceforge.net; Gorski et al.
2005). Some of this work was performed using the Darwin Supercomputer of
the University of Cambridge High Performance Computing Service (http:
//www.hpc.cam.ac.uk/), provided by Dell Inc. using Strategic Research
Infrastructure Funding from the Higher Education Funding Council for
England and funding from the Science and Technology Facilities Council.
NR 126
TC 3
Z9 3
U1 0
U2 0
PU EDP SCIENCES S A
PI LES ULIS CEDEX A
PA 17, AVE DU HOGGAR, PA COURTABOEUF, BP 112, F-91944 LES ULIS CEDEX A,
FRANCE
SN 1432-0746
J9 ASTRON ASTROPHYS
JI Astron. Astrophys.
PD OCT
PY 2016
VL 594
AR A27
DI 10.1051/0004-6361/201525823
PG 38
WC Astronomy & Astrophysics
SC Astronomy & Astrophysics
GA DZ4MG
UT WOS:000385832200010
ER
PT J
AU Ade, PAR
Aghanim, N
Arnaud, M
Aumont, J
Baccigalupi, C
Banday, AJ
Barreiro, RB
Bartlett, JG
Bartolo, N
Battaner, E
Benabed, K
Benoit-Levy, A
Bernard, JP
Bersanelli, M
Bielewicz, P
Bock, JJ
Bonaldi, A
Bonavera, L
Bond, JR
Borrill, J
Bouchet, FR
Burigana, C
Butler, RC
Calabrese, E
Catalano, A
Chamballu, A
Chiang, HC
Christensen, PR
Churazov, E
Clements, DL
Colombo, LPL
Combet, C
Comis, B
Couchot, F
Coulais, A
Crill, BP
Curto, A
Cuttaia, F
Danese, L
Davies, RD
Davis, RJ
de Bernardis, P
de Rosa, A
de Zotti, G
Delabrouille, J
Dickinson, C
Diego, JM
Dole, H
Donzelli, S
Dore, O
Douspis, M
Ducout, A
Dupac, X
Efstathiou, G
Elsner, F
Ensslin, TA
Eriksen, HK
Finelli, F
Flores-Cacho, I
Forni, O
Frailis, M
Fraisse, AA
Franceschi, E
Galeotta, S
Galli, S
Ganga, K
Genova-Santos, RT
Giard, M
Giraud-Heraud, Y
Gjerlow, E
Gonzalez-Nuevo, J
Gorski, KM
Gregorio, A
Gruppuso, A
Gudmundsson, JE
Hansen, FK
Harrison, DL
Helou, G
Hernandez-Monteagudo, C
Herranz, D
Hildebrandt, SR
Hivon, E
Hobson, M
Hornstrup, A
Hovest, W
Huffenberger, KM
Hurier, G
Jaffe, AH
Jaffe, TR
Jones, WC
Keihanen, E
Keskitalo, R
Kisner, TS
Kneissl, R
Knoche, J
Kunz, M
Kurki-Suonio, H
Lagache, G
Lamarre, JM
Langer, M
Lasenby, A
Lattanzi, M
Lawrence, CR
Leonardi, R
Levrier, F
Lilje, PB
Linden-Vornle, M
Lopez-Caniego, M
Lubin, PM
Macias-Perez, JF
Maffei, B
Maggio, G
Maino, D
Mak, DSY
Mandolesi, N
Mangilli, A
Maris, M
Martin, PG
Martinez-Gonzalez, E
Masi, S
Matarrese, S
Melchiorri, A
Mennella, A
Migliaccio, M
Mitra, S
Miville-Deschenes, MA
Moneti, A
Montier, L
Morgante, G
Mortlock, D
Munshi, D
Murphy, JA
Nati, F
Natoli, P
Noviello, F
Novikov, D
Novikov, I
Oxborrow, CA
Paci, F
Pagano, L
Pajot, F
Paoletti, D
Partridge, B
Pasian, F
Pearson, TJ
Perdereau, O
Perotto, L
Pettorino, V
Piacentini, F
Piat, M
Pierpaoli, E
Plaszczynski, S
Pointecouteau, E
Polenta, G
Ponthieu, N
Pratt, GW
Prunet, S
Puget, JL
Rachen, JP
Reinecke, M
Remazeilles, M
Renault, C
Renzi, A
Ristorcelli, I
Rocha, G
Rosset, C
Rossetti, M
Roudier, G
Rubino-Martin, JA
Rusholme, B
Sandri, M
Santos, D
Savelainen, M
Savini, G
Scott, D
Spencer, LD
Stolyarov, V
Stompor, R
Sunyaev, R
Sutton, D
Suur-Uski, AS
Sygnet, JF
Tauber, JA
Terenzi, L
Toffolatti, L
Tomasi, M
Tristram, M
Tucci, M
Umana, G
Valenziano, L
Valiviita, J
Van Tent, B
Vielva, P
Villa, F
Wade, LA
Wandelt, BD
Wehus, IK
Welikala, N
Yvon, D
Zacchei, A
Zonca, A
AF Ade, P. A. R.
Aghanim, N.
Arnaud, M.
Aumont, J.
Baccigalupi, C.
Banday, A. J.
Barreiro, R. B.
Bartlett, J. G.
Bartolo, N.
Battaner, E.
Benabed, K.
Benoit-Levy, A.
Bernard, J. -P.
Bersanelli, M.
Bielewicz, P.
Bock, J. J.
Bonaldi, A.
Bonavera, L.
Bond, J. R.
Borrill, J.
Bouchet, F. R.
Burigana, C.
Butler, R. C.
Calabrese, E.
Catalano, A.
Chamballu, A.
Chiang, H. C.
Christensen, P. R.
Churazov, E.
Clements, D. L.
Colombo, L. P. L.
Combet, C.
Comis, B.
Couchot, F.
Coulais, A.
Crill, B. P.
Curto, A.
Cuttaia, F.
Danese, L.
Davies, R. D.
Davis, R. J.
de Bernardis, P.
de Rosa, A.
de Zotti, G.
Delabrouille, J.
Dickinson, C.
Diego, J. M.
Dole, H.
Donzelli, S.
Dore, O.
Douspis, M.
Ducout, A.
Dupac, X.
Efstathiou, G.
Elsner, F.
Ensslin, T. A.
Eriksen, H. K.
Finelli, F.
Flores-Cacho, I.
Forni, O.
Frailis, M.
Fraisse, A. A.
Franceschi, E.
Galeotta, S.
Galli, S.
Ganga, K.
Genova-Santos, R. T.
Giard, M.
Giraud-Heraud, Y.
Gjerlow, E.
Gonzalez-Nuevo, J.
Gorski, K. M.
Gregorio, A.
Gruppuso, A.
Gudmundsson, J. E.
Hansen, F. K.
Harrison, D. L.
Helou, G.
Hernandez-Monteagudo, C.
Herranz, D.
Hildebrandt, S. R.
Hivon, E.
Hobson, M.
Hornstrup, A.
Hovest, W.
Huffenberger, K. M.
Hurier, G.
Jaffe, A. H.
Jaffe, T. R.
Jones, W. C.
Keihanen, E.
Keskitalo, R.
Kisner, T. S.
Kneissl, R.
Knoche, J.
Kunz, M.
Kurki-Suonio, H.
Lagache, G.
Lamarre, J. -M.
Langer, M.
Lasenby, A.
Lattanzi, M.
Lawrence, C. R.
Leonardi, R.
Levrier, F.
Lilje, P. B.
Linden-Vornle, M.
Lopez-Caniego, M.
Lubin, P. M.
Macias-Perez, J. F.
Maffei, B.
Maggio, G.
Maino, D.
Mak, D. S. Y.
Mandolesi, N.
Mangilli, A.
Maris, M.
Martin, P. G.
Martinez-Gonzalez, E.
Masi, S.
Matarrese, S.
Melchiorri, A.
Mennella, A.
Migliaccio, M.
Mitra, S.
Miville-Deschenes, M. -A.
Moneti, A.
Montier, L.
Morgante, G.
Mortlock, D.
Munshi, D.
Murphy, J. A.
Nati, F.
Natoli, P.
Noviello, F.
Novikov, D.
Novikov, I.
Oxborrow, C. A.
Paci, F.
Pagano, L.
Pajot, F.
Paoletti, D.
Partridge, B.
Pasian, F.
Pearson, T. J.
Perdereau, O.
Perotto, L.
Pettorino, V.
Piacentini, F.
Piat, M.
Pierpaoli, E.
Plaszczynski, S.
Pointecouteau, E.
Polenta, G.
Ponthieu, N.
Pratt, G. W.
Prunet, S.
Puget, J. -L.
Rachen, J. P.
Reinecke, M.
Remazeilles, M.
Renault, C.
Renzi, A.
Ristorcelli, I.
Rocha, G.
Rosset, C.
Rossetti, M.
Roudier, G.
Rubino-Martin, J. A.
Rusholme, B.
Sandri, M.
Santos, D.
Savelainen, M.
Savini, G.
Scott, D.
Spencer, L. D.
Stolyarov, V.
Stompor, R.
Sunyaev, R.
Sutton, D.
Suur-Uski, A. -S.
Sygnet, J. -F.
Tauber, J. A.
Terenzi, L.
Toffolatti, L.
Tomasi, M.
Tristram, M.
Tucci, M.
Umana, G.
Valenziano, L.
Valiviita, J.
Van Tent, B.
Vielva, P.
Villa, F.
Wade, L. A.
Wandelt, B. D.
Wehus, I. K.
Welikala, N.
Yvon, D.
Zacchei, A.
Zonca, A.
CA Planck Collaborartion
TI Planck 2015 results XXIII. The thermal Sunyaev-Zeldovich effect-cosmic
infrared background correlation
SO ASTRONOMY & ASTROPHYSICS
LA English
DT Article
DE galaxies: clusters: general; infrared: galaxies; large-scale structure
of Universe; methods: data analysis
ID SOUTH-POLE TELESCOPE; ANGULAR POWER SPECTRUM; DARK-MATTER HALOES; GALAXY
CLUSTERS; STAR-FORMATION; COSMOLOGICAL PARAMETERS; SUBMILLIMETER
GALAXIES; SZ; ANISOTROPIES; MODEL
AB We use Planck data to detect the cross-correlation between the thermal Sunyaev-Zeldovich (tSZ) effect and the infrared emission from the galaxies that make up the the cosmic infrared background (CIB). We first perform a stacking analysis towards Planck-confirmed galaxy clusters. We detect infrared emission produced by dusty galaxies inside these clusters and demonstrate that the infrared emission is about 50% more extended than the tSZ effect. Modelling the emission with a Navarro-Frenk-White profile, we find that the radial profile concentration parameter is c(500) = 1.00(-0.15)(+0.18). This indicates that infrared galaxies in the outskirts of clusters have higher infrared flux than cluster-core galaxies. We also study the cross-correlation between tSZ and CIB anisotropies, following three alternative approaches based on power spectrum analyses: (i) using a catalogue of confirmed clusters detected in Planck data; (ii) using an all-sky tSZ map built from Planck frequency maps; and (iii) using cross-spectra between Planck frequency maps. With the three different methods, we detect the tSZ-CIB cross-power spectrum at significance levels of (i) 6 sigma; (ii) 3 sigma; and (iii) 4 sigma. We model the tSZ-CIB cross-correlation signature and compare predictions with the measurements. The amplitude of the cross-correlation relative to the fiducial model is A(tSZ-CIB) = 1.2 +/- 0.3. This result is consistent with predictions for the tSZ-CIB cross-correlation assuming the best-fit cosmological model from Planck 2015 results along with the tSZ and CIB scaling relations.
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[Kunz, M.] African Inst Math Sci, 6-8 Melrose Rd, Cape Town, South Africa.
[Polenta, G.] Agenzia Spaziale Italiana Sci Data Ctr, Via Politecn Snc, I-00133 Rome, Italy.
[Lagache, G.] Aix Marseille Univ, CNRS, LAM Lab Astrophys Marseille, UMR 7326, F-13388 Marseille, France.
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[Bartolo, N.; Matarrese, S.] Ist Nazl Fis Nucl, Sez Padova, Via Marzolo 8, I-35131 Padua, Italy.
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[Banday, A. J.; Bernard, J. -P.; Flores-Cacho, I.; Forni, O.; Giard, M.; Jaffe, T. R.; Montier, L.; Pointecouteau, E.; Ristorcelli, I.] Univ Toulouse, UPS OMP, IRAP, F-31028 Toulouse 4, France.
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RP Hurier, G (reprint author), Univ Paris Sud 11, Inst Astrophys Spatiale, CNRS, UMR 8617, Batiment 121, F-91898 Orsay, France.
EM ghurier@ias.u-psud.fr
RI Churazov, Eugene/A-7783-2013; Barreiro, Rita Belen/N-5442-2014;
bonavera, laura/E-9368-2017; Gonzalez-Nuevo, Joaquin/I-3562-2014;
Herranz, Diego/K-9143-2014; Colombo, Loris/J-2415-2016;
OI Langer, Mathieu/0000-0002-9088-2718; Zacchei,
Andrea/0000-0003-0396-1192; Hivon, Eric/0000-0003-1880-2733; Toffolatti,
Luigi/0000-0003-2645-7386; Lilje, Per/0000-0003-4324-7794; Paoletti,
Daniela/0000-0003-4761-6147; Nati, Federico/0000-0002-8307-5088; Savini,
Giorgio/0000-0003-4449-9416; Pierpaoli, Elena/0000-0002-7957-8993;
Kurki-Suonio, Hannu/0000-0002-4618-3063; Barreiro, Rita
Belen/0000-0002-6139-4272; bonavera, laura/0000-0001-8039-3876;
Gonzalez-Nuevo, Joaquin/0000-0003-1354-6822; Herranz,
Diego/0000-0003-4540-1417; Colombo, Loris/0000-0003-4572-7732; TERENZI,
LUCA/0000-0001-9915-6379; Stolyarov, Vladislav/0000-0001-8151-828X;
Valiviita, Jussi/0000-0001-6225-3693; Hurier,
Guillaume/0000-0002-1215-0706
FU ESA; CNES (France); CNRS/INSU-IN2P3-INP (France); ASI (Italy); CNR
(Italy); INAF (Italy); NASA (USA); DoE (USA); STFC (UK); UKSA (UK); CSIC
(Spain); MINECO (Spain); JA (Spain); RES (Spain); Tekes (Finland); AoF
(Finland); CSC (Finland); DLR (Germany); MPG (Germany); CSA (Canada);
DTU Space (Denmark); SER/SSO (Switzerland); RCN (Norway); SFI (Ireland);
FCT/MCTES (Portugal); ERC; PRACE (EU); French Agence Nationale de la
Recherche [ANR-11-BD56-015]
FX The Planck Collaboration acknowledges the support of: ESA; CNES, and
CNRS/INSU-IN2P3-INP (France); ASI, CNR, and INAF (Italy); NASA and DoE
(USA); STFC and UKSA (UK); CSIC, MINECO, JA and RES (Spain); Tekes, AoF,
and CSC (Finland); DLR and MPG (Germany); CSA (Canada); DTU Space
(Denmark); SER/SSO (Switzerland); RCN (Norway); SFI (Ireland); FCT/MCTES
(Portugal); ERC and PRACE (EU). A description of the Planck
Collaboration and a list of its members, indicating which technical or
scientific activities they have been involved in, can be found at
http://www.cosmos.esa.int/web/planck/planck-collaboration. Some of the
results in this paper have been derived using the HEALPix package. We
also acknowledge the support of the French Agence Nationale de la
Recherche under grant ANR-11-BD56-015.
NR 104
TC 1
Z9 1
U1 0
U2 0
PU EDP SCIENCES S A
PI LES ULIS CEDEX A
PA 17, AVE DU HOGGAR, PA COURTABOEUF, BP 112, F-91944 LES ULIS CEDEX A,
FRANCE
SN 1432-0746
J9 ASTRON ASTROPHYS
JI Astron. Astrophys.
PD OCT
PY 2016
VL 594
AR A23
DI 10.1051/0004-6361/201527418
PG 17
WC Astronomy & Astrophysics
SC Astronomy & Astrophysics
GA DZ4MG
UT WOS:000385832200034
ER
PT J
AU Ade, PAR
Aghanim, N
Arnaud, M
Ashdown, M
Aumont, J
Baccigalupi, C
Banday, AJ
Barreiro, RB
Bartolo, N
Battaner, E
Battye, R
Benabed, K
Benoit, A
Benoit-Levy, A
Bernard, JP
Bersanelli, M
Bielewicz, P
Bock, JJ
Bonaldi, A
Bonavera, L
Bond, JR
Borrill, J
Bouchet, FR
Bucher, M
Burigana, C
Butler, RC
Calabrese, E
Cardoso, JF
Catalano, A
Challinor, A
Chamballu, A
Chiang, HC
Christensen, PR
Church, S
Clements, DL
Colombi, S
Colombo, LPL
Combet, C
Couchot, F
Coulais, A
Crill, BP
Curto, A
Cuttaia, F
Danese, L
Davies, RD
Davis, RJ
de Bernardis, P
de Rosa, A
de Zotti, G
Delabrouille, J
Desert, FX
Diego, JM
Dole, H
Donzelli, S
Dore, O
Douspis, M
Ducout, A
Dupac, X
Efstathiou, G
Elsner, F
Ensslin, TA
Eriksen, HK
Fergusson, J
Finelli, F
Forni, O
Frailis, M
Fraisse, AA
Franceschi, E
Frejsel, A
Galeotta, S
Galli, S
Ganga, K
Giard, M
Giraud-Heraud, Y
Gjerlow, E
Gonzalez-Nuevo, J
Gorski, KM
Gratton, S
Gregorio, A
Gruppuso, A
Gudmundsson, JE
Hansen, FK
Hanson, D
Harrison, DL
Heavens, A
Helou, G
Henrot-Versille, S
Hernandez-Monteagudo, C
Herranz, D
Hildebrandt, SR
Hivon, E
Hobson, M
Holmes, WA
Hornstrup, A
Hovest, W
Huang, Z
Huffenberger, KM
Hurier, G
Jaffe, AH
Jaffe, TR
Jones, WC
Juvela, M
Keihanen, E
Keskitalo, R
Kisner, TS
Knoche, J
Kunz, M
Kurki-Suonio, H
Lagache, G
Lahteenmaki, A
Lamarre, JM
Lasenby, A
Lattanzi, M
Lawrence, CR
Leonardi, R
Lesgourgues, J
Levrier, F
Lewis, A
Liguori, M
Lilje, PB
Linden-Vornle, M
Lopez-Caniego, M
Lubin, PM
Ma, YZ
Macias-Perez, JF
Maggio, G
Maino, D
Mandolesi, N
Mangilli, A
Marchini, A
Maris, M
Martin, PG
Martinelli, M
Martinez-Gonzalez, E
Masi, S
Matarrese, S
McGehee, P
Meinhold, PR
Melchiorri, A
Mendes, L
Mennella, A
Migliaccio, M
Mitra, S
Miville-Deschenes, MA
Moneti, A
Montier, L
Morgante, G
Mortlock, D
Moss, A
Munshi, D
Murphy, JA
Narimani, A
Naselsky, P
Nati, F
Natoli, P
Netterfield, CB
Norgaard-Nielsen, HU
Noviello, F
Novikov, D
Novikov, I
Oxborrow, CA
Paci, F
Pagano, L
Pajot, F
Paoletti, D
Pasian, F
Patanchon, G
Pearson, TJ
Perdereau, O
Perotto, L
Perrotta, F
Pettorino, V
Piacentini, F
Piat, M
Pierpaoli, E
Pietrobon, D
Plaszczynski, S
Pointecouteau, E
Polenta, G
Popa, L
Pratt, GW
Prezeau, G
Prunet, S
Puget, JL
Rachen, JP
Reach, WT
Rebolo, R
Reinecke, M
Remazeilles, M
Renault, C
Renzi, A
Ristorcelli, I
Rocha, G
Rosset, C
Rossetti, M
Roudier, G
Rowan-Robinson, M
Rubino-Martin, JA
Rusholme, B
Salvatelli, V
Sandri, M
Santos, D
Savelainen, M
Savini, G
Schaefer, BM
Scott, D
Seiffert, MD
Shellard, EPS
Spencer, LD
Stolyarov, V
Stompor, R
Sudiwala, R
Sunyaev, R
Sutton, D
Suur-Uski, AS
Sygnet, JF
Tauber, JA
Terenzi, L
Toffolatti, L
Tomasi, M
Tristram, M
Tucci, M
Tuovinen, J
Valenziano, L
Valiviita, J
Van Tent, B
Viel, M
Vielva, P
Villa, F
Wade, LA
Wandelt, BD
Wehus, IK
White, M
Yvon, D
Zacchei, A
Zonca, A
AF Ade, P. A. R.
Aghanim, N.
Arnaud, M.
Ashdown, M.
Aumont, J.
Baccigalupi, C.
Banday, A. J.
Barreiro, R. B.
Bartolo, N.
Battaner, E.
Battye, R.
Benabed, K.
Benoit, A.
Benoit-Levy, A.
Bernard, J. -P.
Bersanelli, M.
Bielewicz, P.
Bock, J. J.
Bonaldi, A.
Bonavera, L.
Bond, J. R.
Borrill, J.
Bouchet, F. R.
Bucher, M.
Burigana, C.
Butler, R. C.
Calabrese, E.
Cardoso, J. -F.
Catalano, A.
Challinor, A.
Chamballu, A.
Chiang, H. C.
Christensen, P. R.
Church, S.
Clements, D. L.
Colombi, S.
Colombo, L. P. L.
Combet, C.
Couchot, F.
Coulais, A.
Crill, B. P.
Curto, A.
Cuttaia, F.
Danese, L.
Davies, R. D.
Davis, R. J.
de Bernardis, P.
de Rosa, A.
de Zotti, G.
Delabrouille, J.
Desert, F. -X.
Diego, J. M.
Dole, H.
Donzelli, S.
Dore, O.
Douspis, M.
Ducout, A.
Dupac, X.
Efstathiou, G.
Elsner, F.
Ensslin, T. A.
Eriksen, H. K.
Fergusson, J.
Finelli, F.
Forni, O.
Frailis, M.
Fraisse, A. A.
Franceschi, E.
Frejsel, A.
Galeotta, S.
Galli, S.
Ganga, K.
Giard, M.
Giraud-Heraud, Y.
Gjerlow, E.
Gonzalez-Nuevo, J.
Gorski, K. M.
Gratton, S.
Gregorio, A.
Gruppuso, A.
Gudmundsson, J. E.
Hansen, F. K.
Hanson, D.
Harrison, D. L.
Heavens, A.
Helou, G.
Henrot-Versille, S.
Hernandez-Monteagudo, C.
Herranz, D.
Hildebrandt, S. R.
Hivon, E.
Hobson, M.
Holmes, W. A.
Hornstrup, A.
Hovest, W.
Huang, Z.
Huffenberger, K. M.
Hurier, G.
Jaffe, A. H.
Jaffe, T. R.
Jones, W. C.
Juvela, M.
Keihanen, E.
Keskitalo, R.
Kisner, T. S.
Knoche, J.
Kunz, M.
Kurki-Suonio, H.
Lagache, G.
Lahteenmaki, A.
Lamarre, J. -M.
Lasenby, A.
Lattanzi, M.
Lawrence, C. R.
Leonardi, R.
Lesgourgues, J.
Levrier, F.
Lewis, A.
Liguori, M.
Lilje, P. B.
Linden-Vornle, M.
Lopez-Caniego, M.
Lubin, P. M.
Ma, Y. -Z.
Macias-Perez, J. F.
Maggio, G.
Maino, D.
Mandolesi, N.
Mangilli, A.
Marchini, A.
Maris, M.
Martin, P. G.
Martinelli, M.
Martinez-Gonzalez, E.
Masi, S.
Matarrese, S.
McGehee, P.
Meinhold, P. R.
Melchiorri, A.
Mendes, L.
Mennella, A.
Migliaccio, M.
Mitra, S.
Miville-Deschenes, M. -A.
Moneti, A.
Montier, L.
Morgante, G.
Mortlock, D.
Moss, A.
Munshi, D.
Murphy, J. A.
Narimani, A.
Naselsky, P.
Nati, F.
Natoli, P.
Netterfield, C. B.
Norgaard-Nielsen, H. U.
Noviello, F.
Novikov, D.
Novikov, I.
Oxborrow, C. A.
Paci, F.
Pagano, L.
Pajot, F.
Paoletti, D.
Pasian, F.
Patanchon, G.
Pearson, T. J.
Perdereau, . O.
Perotto, L.
Perrotta, F.
Pettorino, V.
Piacentini, F.
Piat, M.
Pierpaoli, E.
Pietrobon, D.
Plaszczynski, S.
Pointecouteau, E.
Polenta, G.
Popa, L.
Pratt, G. W.
Prezeau, G.
Prunet, S.
Puget, J. -L.
Rachen, J. P.
Reach, W. T.
Rebolo, R.
Reinecke, M.
Remazeilles, M.
Renault, C.
Renzi, A.
Ristorcelli, I.
Rocha, G.
Rosset, C.
Rossetti, M.
Roudier, G.
Rowan-Robinson, M.
Rubino-Martin, J. A.
Rusholme, B.
Salvatelli, V.
Sandri, M.
Santos, D.
Savelainen, M.
Savini, G.
Schaefer, B. M.
Scott, D.
Seiffert, M. D.
Shellard, E. P. S.
Spencer, L. D.
Stolyarov, V.
Stompor, R.
Sudiwala, R.
Sunyaev, R.
Sutton, D.
Suur-Uski, A. -S.
Sygnet, J. -F.
Tauber, J. A.
Terenzi, L.
Toffolatti, L.
Tomasi, M.
Tristram, M.
Tucci, M.
Tuovinen, J.
Valenziano, L.
Valiviita, J.
Van Tent, B.
Viel, M.
Vielva, P.
Villa, F.
Wade, L. A.
Wandelt, B. D.
Wehus, I. K.
White, M.
Yvon, D.
Zacchei, A.
Zonca, A.
CA Planck Collaboration
TI Planck 2015 results XIV. Dark energy and modified gravity
SO ASTRONOMY & ASTROPHYSICS
LA English
DT Article
DE dark energy; cosmic background radiation; cosmology: theory; gravitation
ID BARYON ACOUSTIC-OSCILLATIONS; REDSHIFT-SPACE DISTORTIONS; MATTER POWER
SPECTRUM; COSMOLOGICAL PERTURBATION-THEORY; MAIN GALAXY SAMPLE; HUBBLE
CONSTANT; GROWTH-RATE; CFHTLENS; MODEL; CMB
AB We study the implications of Planck data for models of dark energy (DE) and modified gravity (MG) beyond the standard cosmological constant scenario. We start with cases where the DE only directly affects the background evolution, considering Taylor expansions of the equation of state w(a), as well as principal component analysis and parameterizations related to the potential of a minimally coupled DE scalar field. When estimating the density of DE at early times, we significantly improve present constraints and find that it has to be below similar to 2% (at 95% confidence) of the critical density, even when forced to play a role for z < 50 only. We then move to general parameterizations of the DE or MG perturbations that encompass both effective field theories and the phenomenology of gravitational potentials in MG models. Lastly, we test a range of specific models, such as k-essence, f(R) theories, and coupled DE. In addition to the latest Planck data, for our main analyses, we use background constraints from baryonic acoustic oscillations, type-Ia supernovae, and local measurements of the Hubble constant. We further show the impact of measurements of the cosmological perturbations, such as redshift-space distortions and weak gravitational lensing. These additional probes are important tools for testing MG models and for breaking degeneracies that are still present in the combination of Planck and background data sets. All results that include only background parameterizations (expansion of the equation of state, early DE, general potentials in minimally-coupled scalar fields or principal component analysis) are in agreement with ACDM. When testing models that also change perturbations (even when the background is fixed to ACDM), some tensions appear in a few scenarios: the maximum one found is similar to 2 sigma for Planck TT + lowP when parameterizing observables related to the gravitational potentials with a chosen time dependence; the tension increases to, at most, 3 sigma when external data sets are included. It however disappears when including CMB lensing.
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[Church, S.] Stanford Univ, Dept Phys, Varian Phys Bldg,382 Via Pueblo Mall, Stanford, CA 94305 USA.
[Calabrese, E.] Univ Oxford, Subdept Astrophys, Keble Rd, Oxford OX1 3RH, England.
[Gudmundsson, J. E.] Stockholm Univ, Oskar Klein Ctr Cosmoparticle Phys, Dept Phys, S-10691 Stockholm, Sweden.
[Lesgourgues, J.] CERN, Div Theory, PH TH, CH-1211 Geneva 23, Switzerland.
[Benabed, K.; Benoit-Levy, A.; Colombi, S.; Elsner, F.; Hivon, E.; Prunet, S.; Wandelt, B. D.] Univ Paris 06, UPMC, UMR7095, 98 Bis Blvd Arago, F-75014 Paris, France.
[Schaefer, B. M.] Heidelberg Univ, Inst Theoret Astrophys, Philosophenweg 12, D-69120 Heidelberg, Germany.
[Banday, A. J.; Bernard, J. -P.; Forni, O.; Giard, M.; Jaffe, T. R.; Montier, L.; Pointecouteau, E.; Ristorcelli, I.] Univ Toulouse, UPS OMP, IRAP, F-31028 Toulouse 4, France.
[Reach, W. T.] Univ Space Res Assoc, Stratospher Observ Infrared Astron, MS 232-11, Moffett Field, CA 94035 USA.
[Battaner, E.] Univ Granada, Fac Ciencias, Dept Fis Teor & Cosmos, Granada 18010, Spain.
[Battaner, E.] Univ Granada, Inst Carlos Fis Teor & Comp 1, Granada 18010, Spain.
[Martinelli, M.] Heidelberg Univ, Inst Theoret Phys, Philosophenweg 16, D-69120 Heidelberg, Germany.
[Gorski, K. M.] Univ Warsaw Observ, Aleje Ujazdowskie 4, PL-00478 Warsaw, Poland.
RP Pettorino, V (reprint author), HGSFP, Philosophenweg 16, D-69120 Heidelberg, Germany.; Pettorino, V (reprint author), Heidelberg Univ, Dept Theoret Phys, Philosophenweg 16, D-69120 Heidelberg, Germany.
EM v.pettorino@thphys.uni-heidelberg.de
RI Lahteenmaki, Anne/L-5987-2013; Barreiro, Rita Belen/N-5442-2014;
bonavera, laura/E-9368-2017; Gonzalez-Nuevo, Joaquin/I-3562-2014;
Herranz, Diego/K-9143-2014; Colombo, Loris/J-2415-2016;
OI Juvela, Mika/0000-0002-5809-4834; TERENZI, LUCA/0000-0001-9915-6379;
Reach, William/0000-0001-8362-4094; Valiviita,
Jussi/0000-0001-6225-3693; Piacentini, Francesco/0000-0002-5444-9327;
Toffolatti, Luigi/0000-0003-2645-7386; Lilje, Per/0000-0003-4324-7794;
Nati, Federico/0000-0002-8307-5088; Savini, Giorgio/0000-0003-4449-9416;
Martinelli, Matteo/0000-0002-6943-7732; Pierpaoli,
Elena/0000-0002-7957-8993; Huang, Zhiqi/0000-0002-1506-1063; Barreiro,
Rita Belen/0000-0002-6139-4272; bonavera, laura/0000-0001-8039-3876;
Gonzalez-Nuevo, Joaquin/0000-0003-1354-6822; Herranz,
Diego/0000-0003-4540-1417; Colombo, Loris/0000-0003-4572-7732;
Kurki-Suonio, Hannu/0000-0002-4618-3063; Zacchei,
Andrea/0000-0003-0396-1192; Stolyarov, Vladislav/0000-0001-8151-828X;
Paoletti, Daniela/0000-0003-4761-6147
FU DFG TransRegio TRR33 grant "The Dark Universe"; Swiss NSF; ESA; CNES
(France); CNRS/INSU-IN2P3-INP (France); ASI (Italy); CNR (Italy); INAF
(Italy); NASA (USA); DoE (USA); STFC (UK); UKSA (UK); CSIC (Spain);
MINECO (Spain); JA (Spain); RES (Spain); Tekes (Finland); AoF (Finland);
CSC (Finland); DLR (Germany); MPG (Germany); CSA (Canada); DTU Space
(Denmark); SER/SSO (Switzerland); RCN (Norway); SFI (Ireland); FCT/MCTES
(Portugal); ERC (EU); PRACE (EU)
FX It is a pleasure to thank Luca Amendola, Emilio Bellini, Diego Blas,
Sarah Bridle, Noemi Frusciante, Catherine Heymans, Alireza Hojjati, Bin
Hu, Thomas Kitching, Niall MacCrann, Marco Raveri, Ignacy Sawicki,
Alessandra Silvestri, Fergus Simpson, Christof Wetterich and Gongbo Zhao
for interesting discussions on theories, external data sets and
numerical codes. Part of the analysis for this paper was run on the
Andromeda and Perseus clusters of the University of Geneva and on
WestGrid computers in Canada. We deeply thank Andreas Malaspinas for
invaluable help with the Andromeda and Perseus Clusters. This research
was partly funded by the DFG TransRegio TRR33 grant on "The Dark
Universe" and by the Swiss NSF. The Planck Collaboration acknowledges
the support of: ESA; CNES and CNRS/INSU-IN2P3-INP (France); ASI, CNR,
and INAF (Italy); NASA and DoE (USA); STFC and UKSA (UK); CSIC, MINECO,
JA, and RES (Spain); Tekes, AoF, and CSC (Finland); DLR and MPG
(Germany); CSA (Canada); DTU Space (Denmark); SER/SSO (Switzerland); RCN
(Norway); SFI (Ireland); FCT/MCTES (Portugal); ERC and PRACE (EU). A
description of the Planck Collaboration and a list of its members,
indicating which technical or scientific activities they have been
involved in, can be found at
http://www.cosmos.esa.int/web/planck/planck-collaboration.
NR 189
TC 11
Z9 11
U1 1
U2 1
PU EDP SCIENCES S A
PI LES ULIS CEDEX A
PA 17, AVE DU HOGGAR, PA COURTABOEUF, BP 112, F-91944 LES ULIS CEDEX A,
FRANCE
SN 1432-0746
J9 ASTRON ASTROPHYS
JI Astron. Astrophys.
PD OCT
PY 2016
VL 594
AR A14
DI 10.1051/0004-6361/201525814
PG 31
WC Astronomy & Astrophysics
SC Astronomy & Astrophysics
GA DZ4MG
UT WOS:000385832200005
ER
PT J
AU Ade, PAR
Aghanim, N
Arnaud, M
Ashdown, M
Aumont, J
Baccigalupi, C
Banday, AJ
Barreiro, RB
Bartlett, JG
Bartolo, N
Basak, S
Battaner, E
Benabed, K
Benoit, A
Benoit-Levy, A
Bernard, JP
Bersanelli, M
Bielewicz, P
Bock, JJ
Bonaldi, A
Bonavera, L
Bond, JR
Borrill, J
Bouchet, FR
Boulanger, F
Bucher, M
Burigana, C
Butler, RC
Calabrese, E
Cardoso, JF
Catalano, A
Challinor, A
Chamballu, A
Chiang, HC
Christensen, PR
Church, S
Clements, DL
Colombi, S
Colombo, LPL
Combet, C
Couchot, F
Coulais, A
Crill, BP
Curto, A
Cuttaia, F
Danese, L
Davies, RD
Davis, RJ
de Bernardis, P
de Rosa, A
de Zotti, G
Delabrouille, J
Desert, FX
Diego, JM
Dole, H
Donzelli, S
Dore, O
Douspis, M
Ducout, A
Dunkley, J
Dupac, X
Efstathiou, G
Elsner, F
Ensslin, TA
Eriksen, HK
Fergusson, J
Finelli, F
Forni, O
Frailis, M
Fraisse, AA
Franceschi, E
Frejsel, A
Galeotta, S
Gallin, S
Ganga, K
Giard, M
Giraud-Heraud, Y
Gjerlow, E
Gonzalez-Nuevo, J
Gorski, KM
Gratton, S
Gregorio, A
Gruppuso, A
Gudmundsson, JE
Hansen, FK
Hanson, D
Harrison, DL
Henrot-Versille, S
Hernandez-Monteagudo, C
Herranz, D
Hildebrandt, SR
Hivon, E
Hobson, M
Holmes, WA
Hornstrup, A
Hovest, W
Huffenberger, KM
Hurier, G
Jaffe, AH
Jaffe, TR
Jones, WC
Juvela, M
Keihanen, E
Keskitalo, R
Kisner, TS
Kneissl, R
Knoche, J
Kunz, M
Kurki-Suonio, H
Lagache, G
Lahteenmaki, A
Lamarre, JM
Lasenby, A
Lattanzi, M
Lawrence, CR
Leonardi, R
Lesgourgues, J
Levrier, F
Lewis, A
Liguori, M
Lilje, PB
Linden-Vornle, M
Lopez-Caniego, M
Lubin, PM
Macias-Perez, JF
Maggio, G
Maino, D
Mandolesi, N
Mangilli, A
Maris, M
Martin, PG
Martinez-Gonzalez, E
Masi, S
Matarrese, S
McGehee, P
Meinhold, PR
Melchiorri, A
Mendes, L
Mennella, A
Migliaccio, M
Mitra, S
Miville-Deschenes, MA
Moneti, A
Montier, L
Morgante, G
Mortlock, D
Moss, A
Munshi, D
Murphy, JA
Naselsky, P
Nati, F
Natoli, P
Netterfield, CB
Norgaard-Nielsen, HU
Noviello, F
Novikov, D
Novikov, I
Oxborrow, CA
Paci, F
Pagano, L
Pajot, F
Paoletti, D
Pasian, F
Patanchon, G
Perdereau, O
Perotto, L
Perrotta, F
Pettorino, V
Piacentini, F
Piat, M
Pierpaoli, E
Pietrobon, D
Plaszczynski, S
Pointecouteau, E
Polenta, G
Popa, L
Pratt, GW
Prezeau, G
Prunet, S
Puget, JL
Rachen, JP
Reach, WT
Rebolo, R
Reinecke, M
Remazeilles, M
Renault, C
Renzi, A
Ristorcelli, I
Rocha, G
Rosset, C
Rossetti, M
Roudier, G
Rowan-Robinson, M
Rubino-Martin, JA
Rusholme, B
Sandri, M
Santos, D
Savelainen, M
Savini, G
Scott, D
Seiffert, MD
Shellard, EPS
Spencer, LD
Stolyarov, V
Stompor, R
Sudiwala, R
Sunyaev, R
Sutton, D
Suur-Uski, AS
Sygnet, JF
Tauber, JA
Terenzi, L
Toffolatti, L
Tomasi, M
Tristram, M
Tucci, M
Tuovinen, J
Valenziano, L
Valiviita, J
Van Tent, B
Vielva, P
Villa, F
Wade, LA
Wandelt, BD
Wehus, IK
White, M
Yvon, D
Zacchei, A
Zonca, A
AF Ade, P. A. R.
Aghanim, N.
Arnaud, M.
Ashdown, M.
Aumont, J.
Baccigalupi, C.
Banday, A. J.
Barreiro, R. B.
Bartlett, J. G.
Bartolo, N.
Basak, S.
Battaner, E.
Benabed, K.
Benoit, A.
Benoit-Levy, A.
Bernard, J. -P.
Bersanelli, M.
Bielewicz, P.
Bock, J. J.
Bonaldi, A.
Bonavera, L.
Bond, J. R.
Borrill, J.
Bouchet, F. R.
Boulanger, F.
Bucher, M.
Burigana, C.
Butler, R. C.
Calabrese, E.
Cardoso, J. -F.
Catalano, A.
Challinor, A.
Chamballu, A.
Chiang, H. C.
Christensen, P. R.
Church, S.
Clements, D. L.
Colombi, S.
Colombo, L. P. L.
Combet, C.
Couchot, F.
Coulais, A.
Crill, B. P.
Curto, A.
Cuttaia, F.
Danese, L.
Davies, R. D.
Davis, R. J.
de Bernardis, P.
de Rosa, A.
de Zotti, G.
Delabrouille, J.
Desert, F. -X.
Diego, J. M.
Dole, H.
Donzelli, S.
Dore, O.
Douspis, M.
Ducout, A.
Dunkley, J.
Dupac, X.
Efstathiou, G.
Elsner, F.
Ensslin, T. A.
Eriksen, H. K.
Fergusson, J.
Finelli, F.
Forni, O.
Frailis, M.
Fraisse, A. A.
Franceschi, E.
Frejsel, A.
Galeotta, S.
Gallin, S.
Ganga, K.
Giard, M.
Giraud-Heraud, Y.
Gjerlow, E.
Gonzalez-Nuevo, J.
Gorski, K. M.
Gratton, S.
Gregorio, A.
Gruppuso, A.
Gudmundsson, J. E.
Hansen, F. K.
Hanson, D.
Harrison, D. L.
Henrot-Versille, S.
Hernandez-Monteagudo, C.
Herranz, D.
Hildebrandt, S. R.
Hivon, E.
Hobson, M.
Holmes, W. A.
Hornstrup, A.
Hovest, W.
Huffenberger, K. M.
Hurier, G.
Jaffe, A. H.
Jaffe, T. R.
Jones, W. C.
Juvela, M.
Keihanen, E.
Keskitalo, R.
Kisner, T. S.
Kneissl, R.
Knoche, J.
Kunz, M.
Kurki-Suonio, H.
Lagache, G.
Lahteenmaki, A.
Lamarre, J. -M.
Lasenby, A.
Lattanzi, M.
Lawrence, C. R.
Leonardi, R.
Lesgourgues, J.
Levrier, F.
Lewis, A.
Liguori, M.
Lilje, P. B.
Linden-Vornle, M.
Lopez-Caniego, M.
Lubin, P. M.
Macias-Perez, J. F.
Maggio, G.
Maino, D.
Mandolesi, N.
Mangilli, A.
Maris, M.
Martin, P. G.
Martinez-Gonzalez, E.
Masi, S.
Matarrese, S.
McGehee, P.
Meinhold, P. R.
Melchiorri, A.
Mendes, L.
Mennella, A.
Migliaccio, M.
Mitra, S.
Miville-Deschenes, M. -A.
Moneti, A.
Montier, L.
Morgante, G.
Mortlock, D.
Moss, A.
Munshi, D.
Murphy, J. A.
Naselsky, P.
Nati, F.
Natoli, P.
Netterfield, C. B.
Norgaard-Nielsen, H. U.
Noviello, F.
Novikov, D.
Novikov, I.
Oxborrow, C. A.
Paci, F.
Pagano, L.
Pajot, F.
Paoletti, D.
Pasian, F.
Patanchon, G.
Perdereau, O.
Perotto, L.
Perrotta, F.
Pettorino, V.
Piacentini, F.
Piat, M.
Pierpaoli, E.
Pietrobon, D.
Plaszczynski, S.
Pointecouteau, E.
Polenta, G.
Popa, L.
Pratt, G. W.
Prezeau, G.
Prunet, S.
Puget, J. -L.
Rachen, J. P.
Reach, W. T.
Rebolo, R.
Reinecke, M.
Remazeilles, M.
Renault, C.
Renzi, A.
Ristorcelli, I.
Rocha, G.
Rosset, C.
Rossetti, M.
Roudier, G.
Rowan-Robinson, M.
Rubino-Martin, J. A.
Rusholme, B.
Sandri, M.
Santos, D.
Savelainen, M.
Savini, G.
Scott, D.
Seiffert, M. D.
Shellard, E. P. S.
Spencer, L. D.
Stolyarov, V.
Stompor, R.
Sudiwala, R.
Sunyaev, R.
Sutton, D.
Suur-Uski, A. -S.
Sygnet, J. -F.
Tauber, J. A.
Terenzi, L.
Toffolatti, L.
Tomasi, M.
Tristram, M.
Tucci, M.
Tuovinen, J.
Valenziano, L.
Valiviita, J.
Van Tent, B.
Vielva, P.
Villa, F.
Wade, L. A.
Wandelt, B. D.
Wehus, I. K.
White, M.
Yvon, D.
Zacchei, A.
Zonca, A.
CA Planck Collaboration
TI Planck 2015 results XV. Gravitational lensing
SO ASTRONOMY & ASTROPHYSICS
LA English
DT Article
DE gravitational lensing: weak; cosmological parameters; cosmic background
radiation; large-scale structure of Universe; cosmology: observations
ID BARYON ACOUSTIC-OSCILLATIONS; SOUTH-POLE TELESCOPE; HUBBLE CONSTANT;
POWER SPECTRUM; CMB; GALAXIES; POLARIZATION; TEMPERATURE; EVOLUTION;
DISTANCE
AB We present the most significant measurement of the cosmic microwave background (CMB) lensing potential to date (at a level of 40 sigma), using temperature and polarization data from the Planck 2015 full-mission release. Using a polarization-only estimator, we detect lensing at a significance of 5 sigma. We cross-check the accuracy of our measurement using the wide frequency coverage and complementarity of the temperature and polarization measurements. Public products based on this measurement include an estimate of the lensing potential over approximately 70% of the sky, an estimate of the lensing potential power spectrum in bandpowers for the multipole range 40 <= L <= 400, and an associated likelihood for cosmological parameter constraints. We find good agreement between our measurement of the lensing potential power spectrum and that found in the Lambda CDM model that best fits the Planck temperature and polarization power spectra. Using the lensing likelihood alone we obtain a percent-level measurement of the parameter combination sigma(8) Omega(0.25)(m) = 0.591 +/- 0.021. We combine our determination of the lensing potential with the E-mode polarization, also measured by Planck, to generate an estimate of the lensing B-mode. We show that this lensing B-mode estimate is correlated with the B-modes observed directly by Planck at the expected level and with a statistical significance of 10 sigma, confirming Planck's sensitivity to this known sky signal. We also correlate our lensing potential estimate with the large-scale temperature anisotropies, detecting a cross-correlation at the 3 sigma level, as expected because of dark energy in the concordance Lambda CDM model.
C1 [Bartlett, J. G.; Bucher, M.; Cardoso, J. -F.; Delabrouille, J.; Ganga, K.; Patanchon, G.; Piat, M.; Remazeilles, M.; Rosset, C.; Roudier, G.; Stompor, R.] Univ Paris Diderot, APC, CNRS IN2P3, CEA Lrfu,Observ Paris,Sorbonne Paris Cite, 10 Rue Alice Domon & Leonie Duquet, F-75205 Paris 13, France.
[Lahteenmaki, A.] Aalto Univ, Metsahovi Radio Observ, POB 13000, Aalto 00076, Finland.
[Lahteenmaki, A.] Aalto Univ, Dept Radio Sci & Engn, POB 13000, Aalto 00076, Finland.
[Kunz, M.] African Inst Math Sci, 6-8 Melrose Rd, ZA-7945 Cape Town, South Africa.
[Natoli, P.; Polenta, G.] Agenzia Spaziale Italiana, Sci Data Ctr, Via Politecn Snc, I-00133 Rome, Italy.
[Lagache, G.] Aix Marseille Univ, CNRS, LAM, UMR 7326, F-13388 Marseille, France.
[Ashdown, M.; Curto, A.; Hobson, M.; Lasenby, A.; Stolyarov, V.] Univ Cambridge, Cavendish Lab, Astrophys Grp, JJ Thomson Ave, Cambridge CB3 0HE, England.
[Chiang, H. C.] Univ KwaZulu Natal, Sch Math Stat & Comp Sci, Astrophys & Cosmol Res Unit, Westville Campus,Private Bag X54001, ZA-4000 Durban, South Africa.
[Kneissl, R.] ALMA Santiago Cent Off, Atacama Large Millimeter Submillimeter Array, Alonso Cordova 3107,Vitacura,Casilla 763 0355, Santiago, Chile.
[Leonardi, R.] CGEE, SCS Qd 9,Lote C,Torre C,4 Andar, BR-70308200 Brasilia, DF, Brazil.
[Bond, J. R.; Hanson, D.; Martin, P. G.; Miville-Deschenes, M. -A.] Univ Toronto, CITA, 60 St George St, Toronto, ON M5S 3H8, Canada.
[Banday, A. J.; Bernard, J. -P.; Bielewicz, P.; Forni, O.; Giard, M.; Giraud-Heraud, Y.; Jaffe, T. R.; Montier, L.; Pointecouteau, E.; Ristorcelli, I.] TRAP, CNRS, 9 Ave Colonel Roche,BP 44346, F-31028 Toulouse 4, France.
[Tuovinen, J.] Trinity Coll Dublin, CRANN, Dublin 2, Ireland.
[Bock, J. J.; Crill, B. P.; Dore, O.; Hildebrandt, S. R.; Prezeau, G.; Rocha, G.; Seiffert, M. D.] CALTECH, Pasadena, CA 91125 USA.
[Challinor, A.; Fergusson, J.; Shellard, E. P. S.] Univ Cambridge, DAMTP, Ctr Theoret Cosmol, Wilberforce Rd, Cambridge CB3 0WA, England.
[Hernandez-Monteagudo, C.] CEFCA, Plaza San Juan,1,Planta 2, Teruel 44001, Spain.
[Borrill, J.; Keskitalo, R.] Lawrence Berkeley Natl Lab, Computat Cosmol Ctr, Berkeley, CA 94720 USA.
[Rebolo, R.] CSIC, Plaza Murillo 2, E-28006 Madrid, Spain.
[Chamballu, A.; Yvon, D.] CEA Saclay, DSM Irfu SPP, F-91191 Gif Sur Yvette, France.
[Hornstrup, A.; Linden-Vornle, M.; Norgaard-Nielsen, H. U.; Oxborrow, C. A.] Tech Univ Denmark, Natl Space Inst, DTU Space, Elektrovej 327, DK-2800 Lyngby, Denmark.
[Kunz, M.; Tucci, M.] Univ Geneva, Dept Phys Theor, 24,Quai E Ansermet, CH-1241 Geneva 4, Switzerland.
[Rebolo, R.; Rubino-Martin, J. A.] Univ La Laguna, Dept Astrofis, Tenerife 38206, Spain.
[Gonzalez-Nuevo, J.; Toffolatti, L.] Univ Oviedo, Dept Fis, Avda Calvo Sotelo S-N, Oviedo 33003, Spain.
[Netterfield, C. B.] Univ Toronto, Dept Astron & Astrophys, 50 St George St, Toronto, ON MSR 0A3, Canada.
[Rachen, J. P.] Radboud Univ Nijmegen, Dept Astrophys IMAPP, POB 9010, NL-6500 GL Nijmegen, Netherlands.
[Scott, D.] Univ British Columbia, Dept Phys & Astron, 6224 Agr Rd, Vancouver, BC V6T 1Z4, Canada.
[Colombo, L. P. L.; Pierpaoli, E.] Univ Southern Calif, Dana & David Dornsife Coll Letter Arts & Sci, Dept Phys & Astron, Los Angeles, CA 90089 USA.
[Benoit-Levy, A.; Elsner, F.] UCL, Dept Phys & Astron, London WC1E 6BT, England.
[Lewis, A.] Univ Sussex, Dept Phys & Astron, Brighton BN1 9QH, E Sussex, England.
[Huffenberger, K. M.] Florida State Univ, Dept Phys, Keen Phys Bldg,77 Chieftan Way, Tallahassee, FL 32306 USA.
[Juvela, M.; Keihanen, E.; Kurki-Suonio, H.; Savelainen, M.; Suur-Uski, A. -S.; Valiviita, J.] Univ Helsinki, Dept Phys, Gustaf Hallstromin Katu 2a, Helsinki 00100, Finland.
[Chiang, H. C.; Fraisse, A. A.; Gudmundsson, J. E.; Jones, W. C.; Nati, F.] Princeton Univ, Dept Phys, Princeton, NJ 08544 USA.
[White, M.] Univ Calif Berkeley, Dept Phys, Berkeley, CA 93106 USA.
[Lubin, P. M.; Meinhold, P. R.; Zonca, A.] Univ Calif Santa Barbara, Dept Phys, Santa Barbara, CA 93106 USA.
[Wandelt, B. D.] Univ Illinois, Dept Phys, 1110 West Green St, Urbana, IL 61801 USA.
[Bartolo, N.; Liguori, M.] Univ Padua, Dipartimento Fis & Astron G Galilei, Via Marzolo 8, I-35131 Padua, Italy.
[Burigana, C.; Lattanzi, M.; Mandolesi, N.; Natoli, P.] Univ Ferrara, Dipartimento Fis & Sci Terra, Via Saragat 1, I-44122 Ferrara, Italy.
[de Bernardis, P.; Masi, S.; Matarrese, S.; Melchiorri, A.; Pagano, L.; Piacentini, F.] Univ Roma La Sapienza, Dipartimento Fis, Ple A Moro 2, Rome, Italy.
[Bersanelli, M.; Maino, D.; Mennella, A.; Rossetti, M.; Tomasi, M.] Univ Milan, Dipartimento Fis, Via Celoria 16, Milan, Italy.
[Gregorio, A.] Univ Trieste, Dipartimento Fis, Via A Valerio 2, Trieste, Italy.
[Renzi, A.] Univ Roma Tor Vergata, Dipartimento Matemat, Via Ric Sci 1, Rome, Italy.
[Christensen, P. R.] Niels Bohr Inst, Discovery Ctr, Blegdamsvej 17, Copenhagen, Denmark.
[Kneissl, R.] European Southern Observ, ESO Vitacura, Alonso Cordova 3107,Vitacura,Casilla 19001, Santiago, Chile.
[Dupac, X.; Lopez-Caniego, M.; Mendes, L.] European Space Agcy, ESAC, Planck Sci Off, Camino Bajo Castillo S-N, Madrid 28692, Spain.
[Tauber, J. A.] European Space Agcy, Estec, Keplerlaan 1, NL-2201 AZ Noordwijk, Netherlands.
[Terenzi, L.] Univ E Campus, Fac Ingn, Via Isimbardi 10, I-22060 Novedrate, CO, Italy.
[Matarrese, S.] Ist Nazl Fis Nucl, Gran Sasso Sci Inst, Viale F Crispi 7, I-67100 Laquila, Italy.
[Pettorino, V.] HGSFP, Philosophenweg 16, D-69120 Heidelberg, Germany.
[Pettorino, V.] Heidelberg Univ, Dept Theoret Phys, Philosophenweg 16, D-69120 Heidelberg, Germany.
[Kurki-Suonio, H.; Lahteenmaki, A.; Savelainen, M.; Suur-Uski, A. -S.; Valiviita, J.] Univ Helsinki, Helsinki Inst Phys, Gustaf Hallstromin Katu 2, Helsinki, Finland.
[de Zotti, G.] INAF Osservatorio Astron Padova, Vicolo Osservatorio 5, I-35141 Padua, Italy.
[Polenta, G.] INAF Osservatorio Astron Roma, Via Frascati 33, I-00136 Rome, Italy.
[Frailis, M.; Galeotta, S.; Gregorio, A.; Maggio, G.; Maris, M.; Pasian, F.; Zacchei, A.] INAF Osservatorio Astron Trieste, Via GB Tiepolo 11, I-34131 Trieste, Italy.
[Burigana, C.; Butler, R. C.; Cuttaia, F.; de Rosa, A.; Finelli, F.; Franceschi, E.; Gruppuso, A.; Mandolesi, N.; Morgante, G.; Natoli, P.; Paoletti, D.; Sandri, M.; Terenzi, L.; Toffolatti, L.; Valenziano, L.; Villa, F.] INAF IASF Bologna, Via Gobetti 101, I-40127 Bologna, Italy.
[Bersanelli, M.; Donzelli, S.; Maino, D.; Mennella, A.; Rossetti, M.; Tomasi, M.] INAF IASF Milano, Via E Bassini 15,28, Milan, Italy.
[Burigana, C.; Finelli, F.; Paoletti, D.] Ist Nazl Fis Nucl, Sez Bologna, Via Irnerio 46, I-40126 Bologna, Italy.
[Melchiorri, A.; Pagano, L.] Univ Roma Sapienza, Ist Nazl Fis Nucl, Sez Roma 1, Piazzale Aldo Moro 2, I-00185 Rome, Italy.
[Renzi, A.] Univ Roma Tor Vergata, Sez Roma 2, Ist Nazl Fis Nucl, Via Ric Sci 1, Rome, Italy.
[Gregorio, A.] INFN Natl Inst Nucl Phys, Via Valerio 2, I-34127 Trieste, Italy.
[Desert, F. -X.] Univ Grenoble Alpes, IPAG, F-38000 Grenoble, France.
[Desert, F. -X.] IPAG, CNRS, F-38000 Grenoble, France.
[Mitra, S.] IUCAA, Post Bag 4,Pune Univ Campus, Pune 411007, Maharashtra, India.
[Clements, D. L.; Ducout, A.; Jaffe, A. H.; Mortlock, D.; Rowan-Robinson, M.] Imperial Coll London, Astrophys Grp, Blackett Lab, Prince Consort Rd, London SW7 2AZ, England.
[McGehee, P.; Rusholme, B.] CALTECH, Infrared Proc & Anal Ctr, Pasadena, CA 91125 USA.
[Benoit, A.] Univ Joseph Fourier Grenoble I, Inst Neel, CNRS, 25 Rue Martyrs, F-38401 Grenoble, France.
[Dole, H.; Lagache, G.] Inst Univ France, 103 Bd St Michel, F-75005 Paris, France.
[Aghanim, N.; Aumont, J.; Boulanger, F.; Chamballu, A.; Dole, H.; Douspis, M.; Hurier, G.; Kunz, M.; Mangilli, A.; Miville-Deschenes, M. -A.; Pajot, F.; Puget, J. -L.; Remazeilles, M.] Univ Paris Sud 11, CNRS, Inst Astrophys Spatiale, UMR8617, Batiment 121, F-91400 Orsay, France.
[Benabed, K.; Benoit-Levy, A.; Bouchet, F. R.; Cardoso, J. -F.; Colombi, S.; Ducout, A.; Elsner, F.; Hivon, E.; Moneti, A.; Prunet, S.; Sygnet, J. -F.; Wandelt, B. D.] Inst Astrophys Paris, CNRS, UMR7095, 98 Bis Blvd Arago, F-75014 Paris, France.
[Lesgourgues, J.] Rhein Westfal TH Aachen, Inst Theoret Teilchenphys & Kosmol, D-52056 Aachen, Germany.
[Popa, L.] Inst Space Sci, Bucharest 077125, Romania.
[Challinor, A.; Efstathiou, G.; Harrison, D. L.; Migliaccio, M.; Sutton, D.] Univ Cambridge, Inst Astron, Madingley Rd, Cambridge CB3 0HA, England.
[Eriksen, H. K.; Gjerlow, E.; Hansen, F. K.; Lilje, P. B.] Univ Oslo, Inst Theoret Astrophys, N-0316 Oslo, Norway.
[Rebolo, R.; Rubino-Martin, J. A.] Inst Astrofis Canarias, C Via Lactea S-N, Tenerife 38205, Spain.
[Barreiro, R. B.; Bonavera, L.; Curto, A.; Diego, J. M.; Gonzalez-Nuevo, J.; Herranz, D.; Lopez-Caniego, M.; Martinez-Gonzalez, E.; Toffolatti, L.; Vielva, P.] Univ Cantabria, CSIC, Inst Fis Cantabria, Avda Castros S-N, Santander, Spain.
[Bartolo, N.; Liguori, M.; Matarrese, S.] Ist Nazl Fis Nucl, Sez Padova, Via Marzolo 8, I-35131 Padua, Italy.
[Bartlett, J. G.; Bock, J. J.; Colombo, L. P. L.; Crill, B. P.; Dore, O.; Gorski, K. M.; Hanson, D.; Hildebrandt, S. R.; Holmes, W. A.; Lawrence, C. R.; Mitra, S.; Pietrobon, D.; Prezeau, G.; Rocha, G.; Roudier, G.; Seiffert, M. D.; Wade, L. A.; Wehus, I. K.] CALTECH, Jet Prop Lab, 4800 Oak Grove Dr, Pasadena, CA 91125 USA.
[Bonaldi, A.; Davies, R. D.; Davis, R. J.; Noviello, F.; Remazeilles, M.] Univ Manchester, Sch Phys & Astron, Jodrell Bank Ctr Astrophys, Alan Turing Bldg,Oxford Rd, Manchester M13 9PL, Lancs, England.
[Gallin, S.] Univ Chicago, Kavli Inst Cosmol Phys, Chicago, IL 60637 USA.
[Ashdown, M.; Challinor, A.; Curto, A.; Gratton, S.; Harrison, D. L.; Lasenby, A.; Migliaccio, M.; Sutton, D.] Kavli Inst Cosmol Cambridge, Madingley Rd, Cambridge CB3 0HA, England.
[Stolyarov, V.] Kazan Fed Univ, 18 Kremlyovskaya St, Kazan 420008, Russia.
[Couchot, F.; Henrot-Versille, S.; Mangilli, A.; Perdereau, O.; Plaszczynski, S.; Tristram, M.] Univ Paris 11, CNRS IN2P3, LAL, F-91400 Orsay, France.
[Catalano, A.; Coulais, A.; Lamarre, J. -M.; Levrier, F.; Roudier, G.] Observ Paris, CNRS, LERMA, 61 Ave Observ, F-75014 Paris, France.
[Arnaud, M.; Chamballu, A.; Pratt, G. W.] Univ Paris Diderot, CEA DSM, Lab AIM, IRFU Serv Astrophys,CNRS,CEA Saclay, Bat 709, F-91191 Gif Sur Yvette, France.
[Cardoso, J. -F.] CNRS, Lab Traitement & Commun Informat, UMR 5141, 46 Rue Barrault, F-75634 Paris 13, France.
[Cardoso, J. -F.] Telecom ParisTech, 46 Rue Barrault, F-75634 Paris 13, France.
[Catalano, A.; Combet, C.; Macias-Perez, J. F.; Perotto, L.; Renault, C.; Santos, D.] Univ Grenoble Alpes, CNRS IN2P3, Lab Phys Subat & Cosmol, 53 Rue Martyrs, F-38026 Grenoble, France.
[Van Tent, B.] Univ Paris Sud 11, Lab Phys Theor, Bailment 210, F-91405 Orsay, France.
[Van Tent, B.] CNRS, Bailment 210, F-91405 Orsay, France.
[Kisner, T. S.] Lawrence Berkeley Natl Lab, Berkeley, CA 94720 USA.
[Novikov, D.; Novikov, I.] Russian Acad Sci, Lebedev Phys Inst, Ctr Astro Space, 84-32 Profsoyuznaya St,GSP 7, Moscow 117997, Russia.
[Ensslin, T. A.; Hernandez-Monteagudo, C.; Hovest, W.; Knoche, J.; Rachen, J. P.; Reinecke, M.; Sunyaev, R.] Max Planck Inst Astrophys, Karl Schwarzschild Str 1, D-85741 Garching, Germany.
[Hanson, D.] McGill Univ, McGill Phys, Ernest Rutherford Phys Bldg,3600 Rue Univ, Montreal, PQ H3A 2T8, Canada.
[Murphy, J. A.] Natl Univ Ireland, Dept Expt Phys, Maynooth, Kildare, Ireland.
[Bielewicz, P.] Nicolaus Copernicus Astron Ctr, Bartycka 18, PL-00716 Warsaw, Poland.
[Christensen, P. R.; Frejsel, A.; Novikov, I.] Niels Bohr Inst, Blegdamsvej 17, DK-2100 Copenhagen, Denmark.
[Naselsky, P.] Univ Copenhagen, Niels Bohr Inst, Blegdamsvej 17, DK-2100 Copenhagen, Denmark.
[Gudmundsson, J. E.] Nordita Nord Inst Theoret Phys, Roslagstullsbacken 23, S-10691 Stockholm, Sweden.
[Savini, G.] UCL, Opt Sci Lab, London WC1E 6BT, England.
[Baccigalupi, C.; Basak, S.; Bielewicz, P.; Danese, L.; de Zotti, G.; Paci, F.; Perrotta, F.] SISSA, Astrophys Sect, Via Bonomea 265, I-34136 Trieste, Italy.
[Ade, P. A. R.; Munshi, D.; Spencer, L. D.; Sudiwala, R.] Cardiff Univ, Sch Phys & Astron, Queens Bldg, Cardiff CF24 3AA, S Glam, Wales.
[Moss, A.] Univ Nottingham, Sch Phys & Astron, Nottingham NG7 2RD, England.
[Bouchet, F. R.] Sorbonne Univ UPMC, UMR7095, Inst Astrophys Paris, 98 Bis Blvd Arago, F-75014 Paris, France.
[Sunyaev, R.] Russian Acad Sci, Space Res Inst IKI, Profsoyuznaya Str 84-32, Moscow 117997, Russia.
[Borrill, J.] Univ Calif Berkeley, Space Sci Lab, Berkeley, CA 94720 USA.
[Stolyarov, V.] Russian Acad Sci, Special Astrophys Observ, Karachai Cherkessian Rep 369167, Zelenchukskiy R, Russia.
[Church, S.] Stanford Univ, Dept Phys, Varian Phys Bldg,382 Via Pueblo Mall, Stanford, CA 94305 USA.
[Calabrese, E.; Dunkley, J.] Univ Oxford, Subdept Astrophys, Keble Rd, Oxford OX1 3RH, England.
[Gudmundsson, J. E.] Stockholm Univ, Dept Phys, Oskar Klein Ctr Cosmoparticle Phys, S-10691 Stockholm, Sweden.
[Lesgourgues, J.] CERN, PH TH, Div Theory, CH-1211 Geneva 23, Switzerland.
[Benabed, K.; Benoit-Levy, A.; Colombi, S.; Elsner, F.; Hivon, E.; Prunet, S.; Wandelt, B. D.] UPMC Univ Paris 06, UMR7095, 98 Bis Blvd Arago, F-75014 Paris, France.
[Banday, A. J.; Bernard, J. -P.; Forni, O.; Giard, M.; Jaffe, T. R.; Montier, L.; Pointecouteau, E.; Ristorcelli, I.] Univ Toulouse, UPS OMP, IRAP, F-31028 Toulouse 4, France.
[Reach, W. T.] Univ Space Res Assoc, Stratospher Observ Infrared Astron, MS 232-11, Moffett Field, CA 94035 USA.
[Battaner, E.] Univ Granada, Dept Fis Teer & Cosmos, Granada 18010, Spain.
[Battaner, E.] Univ Granada, Inst Carlos Fis Teer & Computac 1, Granada 18010, Spain.
[Gorski, K. M.] Univ Warsaw Observ, Aleje Ujazdowskie 4, PL-00478 Warsaw, Poland.
RP Hanson, D (reprint author), Univ Toronto, CITA, 60 St George St, Toronto, ON M5S 3H8, Canada.; Hanson, D (reprint author), CALTECH, Jet Prop Lab, 4800 Oak Grove Dr, Pasadena, CA 91125 USA.; Hanson, D (reprint author), McGill Univ, McGill Phys, Ernest Rutherford Phys Bldg,3600 Rue Univ, Montreal, PQ H3A 2T8, Canada.
EM duncan.hanson@gmail.com
RI Lahteenmaki, Anne/L-5987-2013; Barreiro, Rita Belen/N-5442-2014;
bonavera, laura/E-9368-2017; Gonzalez-Nuevo, Joaquin/I-3562-2014;
Herranz, Diego/K-9143-2014; Colombo, Loris/J-2415-2016;
OI Juvela, Mika/0000-0002-5809-4834; Barreiro, Rita
Belen/0000-0002-6139-4272; bonavera, laura/0000-0001-8039-3876;
Gonzalez-Nuevo, Joaquin/0000-0003-1354-6822; Herranz,
Diego/0000-0003-4540-1417; Colombo, Loris/0000-0003-4572-7732;
Valiviita, Jussi/0000-0001-6225-3693; Hivon, Eric/0000-0003-1880-2733;
Kurki-Suonio, Hannu/0000-0002-4618-3063; Zacchei,
Andrea/0000-0003-0396-1192; Stolyarov, Vladislav/0000-0001-8151-828X;
Paoletti, Daniela/0000-0003-4761-6147; TERENZI,
LUCA/0000-0001-9915-6379; Reach, William/0000-0001-8362-4094;
Toffolatti, Luigi/0000-0003-2645-7386; Lilje, Per/0000-0003-4324-7794;
Nati, Federico/0000-0002-8307-5088; Savini, Giorgio/0000-0003-4449-9416;
Pierpaoli, Elena/0000-0002-7957-8993
FU ESA; CNES (France); CNRS/INSU-IN2P3-INP (France); ASI (Italy); CNR
(Italy); INAF (Italy); NASA (USA); DoE (USA); STFC (UK); UKSA (UK); CSIC
(Spain); MINECO (Spain); JA (Spain); RES (Spain); Tekes (Finland); AoF
(Finland); CSC (Finland); DLR (Germany); MPG (Germany); CSA (Canada);
DTU Space (Denmark); SER/SSO (Switzerland); RCN (Norway); SFI (Ireland);
FCT/MCTES (Portugal); ERC (EU); PRACE (EU); Science and Technology
Facilities Council [ST/L000652/1]; European Research Council under the
European Union's Seventh Framework Programme (FP)/ERC Grant [616170]; UK
BIS National E-infrastructure capital grants
FX The Planck Collaboration acknowledges the support of: ESA; CNES and
CNRS/INSU-IN2P3-INP (France); ASI, CNR, and INAF (Italy); NASA and DoE
(USA); STFC and UKSA (UK); CSIC, MINECO, JA, and RES (Spain); Tekes,
AoF, and CSC (Finland); DLR and MPG (Germany); CSA (Canada); DTU Space
(Denmark); SER/SSO (Switzerland); RCN (Norway); SFI (Ireland); FCT/MCTES
(Portugal); ERC and PRACE (EU). A description of the Planck
Collaboration and a list of its members, indicating which technical or
scientific activities they have been involved in, can be found at
http://www.cosmos.esa.int/web/planck/planck-collaboration. Some of the
results in this paper have been derived using the HEALPix package. We
acknowledge support from the Science and Technology Facilities Council
[grant number ST/L000652/1]. The research leading to these results has
received funding from the European Research Council under the European
Union's Seventh Framework Programme (FP/2007-2013)/ERC Grant Agreement
No. [616170]. Part of this work was undertaken on the STFC DiRAC HPC
Facilities at the University of Cambridge funded by UK BIS National
E-infrastructure capital grants.
NR 79
TC 10
Z9 10
U1 1
U2 1
PU EDP SCIENCES S A
PI LES ULIS CEDEX A
PA 17, AVE DU HOGGAR, PA COURTABOEUF, BP 112, F-91944 LES ULIS CEDEX A,
FRANCE
SN 1432-0746
J9 ASTRON ASTROPHYS
JI Astron. Astrophys.
PD OCT
PY 2016
VL 594
AR A15
DI 10.1051/0004-6361/201525941
PG 28
WC Astronomy & Astrophysics
SC Astronomy & Astrophysics
GA DZ4MG
UT WOS:000385832200020
ER
PT J
AU Ade, PAR
Aghanim, N
Arnaud, M
Ashdown, M
Aumont, J
Baccigalupi, C
Banday, AJ
Barreiro, RB
Bartolo, N
Basak, S
Battaner, E
Benabed, K
Benoit, A
Benoit-Levy, A
Bernard, JP
Bersanelli, M
Bielewicz, P
Bock, JJ
Bonaldi, A
Bonavera, L
Bond, JR
Borri, J
Bouchet, FR
Bucher, M
Burigana, C
Butler, RC
Calabrese, E
Cardoso, JF
Casaponsa, B
Catalano, A
Challinor, A
Chamballu, A
Chiang, HC
Christensen, PR
Church, S
Clements, DL
Colombi, S
Colombo, LPL
Combet, C
Couchot, F
Coulais, A
Crill, BP
Curto, A
Cuttaia, F
Danese, L
Davies, RD
Davis, RJ
de Bernardis, P
de Rosa, A
de Zotti, G
Delabrouille, J
Desert, FX
Diego, JM
Dole, H
Donzelli, S
Dore, O
Douspis, M
Ducout, A
Dupac, X
Efstathiou, G
Elsner, F
Ensslin, TA
Eriksen, HK
Fergusson, J
Fernandez-Cobos, R
Finelli, F
Forni, O
Frailis, M
Fraisse, AA
Franceschi, E
Frejsel, A
Galeotta, S
Galli, S
Ganga, K
Genova-Santos, RT
Girad, M
Giraud-Heraud, Y
Gjerlow, E
Gonzalez-Nuevo, J
Gorski, KM
Gratton, S
Gregorio, A
Gruppuso, A
Gudmundsson, JE
Hansen, FK
Hanson, D
Harrison, DL
Henrot-Versille, S
Hernandez-Monteagudo, C
Herranz, D
Hildebrandt, SR
Hivon, E
Hobson, M
Holmes, WA
Hornstrup, A
Hovest, W
Huffenberger, KM
Hurier, G
Ilic, S
Jaffe, AH
Jaffe, TR
Jones, WC
Juvela, M
Keihanen, E
Keskitalo, R
Kisner, TS
Kneiss, R
Knoche, J
Kunz, M
Kurki-Suonio, H
Lagache, G
Lahteenmaki, A
Lamarre, JM
Langer, M
Lasenby, A
Lattanzi, M
Lawrence, CR
Leonardi, R
Lesgourgues, J
Levrier, F
Liguori, M
Lilje, PB
Linden-Vornle, M
Lopez-Caniego, M
Lubin, PM
Ma, YZ
Macias-Perez, JF
Maggio, G
Maino, D
Mandolesi, N
Mangilli, A
Marcos-Caballero, A
Maris, M
Martin, PG
Martinez-Gonzalez, E
Masi, S
Matarrese, S
McGehee, P
Meinhold, PR
Melchiorri, A
Mendes, L
Mennella, A
Migliaccio, M
Mitra, S
Miville-Deschenes, MA
Moneti, A
Montier, L
Morgante, G
Mortlock, D
Moss, A
Munshi, D
Murphy, JA
Naselsky, P
Nati, F
Natoli, P
Netterfield, CB
Norgaard-Nielsen, HU
Noviello, F
Novikov, D
Novikov, I
Oxborrow, CA
Paci, F
Pagano, L
Pajot, F
Paoletti, D
Pasian, F
Patanchon, G
Perdereau, O
Perotto, L
Perrotta, F
Pettorino, V
Piacentini, F
Piat, M
Pierpaoli, E
Pietrobon, D
Plaszczynski, S
Pointecouteau, E
Polenta, G
Popa, L
Pratt, GW
Prezeau, G
Prunet, S
Puget, JL
Rachen, JP
Reach, WT
Rebolo, R
Reinecke, M
Remazeilles, M
Renault, C
Renzi, A
Ristorcelli, I
Rocha, G
Rosset, C
Rossetti, M
Roudier, G
Rubino-Martin, JA
Rusholme, B
Sandri, M
Santos, D
Savelainen, M
Savini, G
Schaefer, BM
Scott, D
Seiffert, MD
Shellard, EPS
Spencer, LD
Stolyarov, V
Stompor, R
Sudiwala, R
Sunyaev, R
Sutton, D
Suur-Uski, AS
Sygnet, JF
Tauber, JA
Terenzi, L
Toffolatti, L
Tomasi, M
Tristram, M
Tucci, M
Tuovinen, J
Valenziano, L
Valiviita, J
Van Tent, F
Vielva, P
Villa, F
Wade, LA
Wandelt, BD
Wehus, IK
Yvon, D
Zacchei, A
Zonca, A
AF Ade, P. A. R.
Aghanim, N.
Arnaud, M.
Ashdown, M.
Aumont, J.
Baccigalupi, C.
Banday, A. J.
Barreiro, R. B.
Bartolo, N.
Basak, S.
Battaner, E.
Benabed, K.
Benoit, A.
Benoit-Levy, A.
Bernard, J. -P.
Bersanelli, M.
Bielewicz, P.
Bock, J. J.
Bonaldi, A.
Bonavera, L.
Bond, J. R.
Borri, J.
Bouchet, F. R.
Bucher, M.
Burigana, C.
Butler, R. C.
Calabrese, E.
Cardoso, J. -F.
Casaponsa, B.
Catalano, A.
Challinor, A.
Chamballu, A.
Chiang, H. C.
Christensen, P. R.
Church, S.
Clements, D. L.
Colombi, S.
Colombo, L. P. L.
Combet, C.
Couchot, F.
Coulais, A.
Crill, B. P.
Curto, A.
Cuttaia, F.
Danese, L.
Davies, R. D.
Davis, R. J.
de Bernardis, P.
de Rosa, A.
de Zotti, G.
Delabrouille, J.
Desert, F. -X.
Diego, J. M.
Dole, H.
Donzelli, S.
Dore, O.
Douspis, M.
Ducout, A.
Dupac, X.
Efstathiou, G.
Elsner, F.
Ensslin, T. A.
Eriksen, H. K.
Fergusson, J.
Fernandez-Cobos, R.
Finelli, F.
Forni, O.
Frailis, M.
Fraisse, A. A.
Franceschi, E.
Frejsel, A.
Galeotta, S.
Galli, S.
Ganga, K.
Genova-Santos, R. T.
Girad, M.
Giraud-Heraud, Y.
Gjerlow, E.
Gonzalez-Nuevo, J.
Gorski, K. M.
Gratton, S.
Gregorio, A.
Gruppuso, A.
Gudmundsson, J. E.
Hansen, F. K.
Hanson, D.
Harrison, D. L.
Henrot-Versille, S.
Hernandez-Monteagudo, C.
Herranz, D.
Hildebrandt, S. R.
Hivon, E.
Hobson, M.
Holmes, W. A.
Hornstrup, A.
Hovest, W.
Huffenberger, K. M.
Hurier, G.
Ilic, S.
Jaffe, A. H.
Jaffe, T. R.
Jones, W. C.
Juvela, M.
Keihanen, E.
Keskitalo, R.
Kisner, T. S.
Kneiss, R.
Knoche, J.
Kunz, M.
Kurki-Suonio, H.
Lagache, G.
Lahteenmaki, A.
Lamarre, J. -M.
Langer, M.
Lasenby, A.
Lattanzi, M.
Lawrence, C. R.
Leonardi, R.
Lesgourgues, J.
Levrier, F.
Liguori, M.
Lilje, P. B.
Linden-Vornle, M.
Lopez-Caniego, M.
Lubin, P. M.
Ma, Y. -Z.
Macias-Perez, J. F.
Maggio, G.
Maino, D.
Mandolesi, N.
Mangilli, A.
Marcos-Caballero, A.
Maris, M.
Martin, P. G.
Martinez-Gonzalez, E.
Masi, S.
Matarrese, S.
McGehee, P.
Meinhold, P. R.
Melchiorri, A.
Mendes, L.
Mennella, A.
Migliaccio, M.
Mitra, S.
Miville-Deschenes, M. -A.
Moneti, A.
Montier, L.
Morgante, G.
Mortlock, D.
Moss, A.
Munshi, D.
Murphy, J. A.
Naselsky, P.
Nati, F.
Natoli, P.
Netterfield, C. B.
Norgaard-Nielsen, H. U.
Noviello, F.
Novikov, D.
Novikov, I.
Oxborrow, C. A.
Paci, F.
Pagano, L.
Pajot, F.
Paoletti, D.
Pasian, F.
Patanchon, G.
Perdereau, O.
Perotto, L.
Perrotta, F.
Pettorino, V.
Piacentini, F.
Piat, M.
Pierpaoli, E.
Pietrobon, D.
Plaszczynski, S.
Pointecouteau, E.
Polenta, G.
Popa, L.
Pratt, G. W.
Prezeau, G.
Prunet, S.
Puget, J. -L.
Rachen, J. P.
Reach, W. T.
Rebolo, R.
Reinecke, M.
Remazeilles, M.
Renault, C.
Renzi, A.
Ristorcelli, I.
Rocha, G.
Rosset, C.
Rossetti, M.
Roudier, G.
Rubino-Martin, J. A.
Rusholme, B.
Sandri, M.
Santos, D.
Savelainen, M.
Savini, G.
Schaefer, B. M.
Scott, D.
Seiffert, M. D.
Shellard, E. P. S.
Spencer, L. D.
Stolyarov, V.
Stompor, R.
Sudiwala, R.
Sunyaev, R.
Sutton, D.
Suur-Uski, A. -S.
Sygnet, J. -F.
Tauber, J. A.
Terenzi, L.
Toffolatti, L.
Tomasi, M.
Tristram, M.
Tucci, M.
Tuovinen, J.
Valenziano, L.
Valiviita, J.
Van Tent, F.
Vielva, P.
Villa, F.
Wade, L. A.
Wandelt, B. D.
Wehus, I. K.
Yvon, D.
Zacchei, A.
Zonca, A.
CA Planck Collaboration
TI XXI. The integrated Sachs-Wolfe effect
SO ASTRONOMY & ASTROPHYSICS
LA English
DT Article
DE cosmology: observations; cosmic background radiation; large-scale
structure of Universe; dark energy; galaxies: clusters: general;
methods: data analysis
ID PROBE WMAP OBSERVATIONS; LARGE-SCALE STRUCTURE; MICROWAVE BACKGROUND
ANOMALIES; DARK ENERGY CONSTRAINTS; DIGITAL SKY SURVEY;
CROSS-CORRELATION; DATA RELEASE; FINDING ALGORITHM; REDSHIFT SURVEY;
POWER SPECTRUM
AB This paper presents a study of the integrated Sachs-Wolfe (ISW) effect from the Planck 2015 temperature and polarization data release. This secondary cosmic microwave background (CMB) anisotropy caused by the large-scale time-evolving gravitational potential is probed from different perspectives. The CMB is cross-correlated with different large-scale structure (LSS) tracers: radio sources from the NVSS catalogue; galaxies from the optical SDSS and the infrared WISE surveys; and the Planck 2015 convergence lensing map. The joint cross-correlation of the CMB with the tracers yields a detection at 4 sigma where most of the signal-to-noise is due to the Planck lensing and the NVSS radio catalogue. In fact, the ISW effect is detected from the Planck data only at approximate to 3 sigma (through the ISW-lensing bispectrum), which is similar to the detection level achieved by combining the cross-correlation signal coming from all the galaxy catalogues mentioned above. We study the ability of the ISW effect to place constraints on the dark-energy parameters; in particular, we show that Omega(Lambda) is detected at more than 3 sigma. This cross-correlation analysis is performed only with the Planck temperature data, since the polarization scales available in the 2015 release do not permit significant improvement of the CMB-LSS cross-correlation detectability. Nevertheless, the Planck polarization data are used to study the anomalously large ISW signal previously reported through the aperture photometry on stacked CMB features at the locations of known superclusters and supervoids, which is in conflict with Lambda CDM expectations. We find that the current Planck polarization data do not exclude that this signal could be caused by the ISW effect. In addition, the stacking of the Planck lensing map on the locations of superstructures exhibits a positive cross-correlation with these large-scale structures. Finally, we have improved our previous reconstruction of the ISW temperature fluctuations by combining the information encoded in all the previously mentioned LSS tracers. In particular, we construct a map of the ISW secondary anisotropies and the corresponding uncertainties map, obtained from simulations. We also explore the reconstruction of the ISW anisotropies caused by the large-scale structure traced by the 2MASS Photometric Redshift Survey (2MPZ) by directly inverting the density field into the gravitational potential field.
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RP Vielva, P (reprint author), Univ Cantabria, CSIC, Inst Fis Cantabria, Avda Castros S-N, Santander 39005, Spain.
EM vielva@ifca.unican.es
RI Barreiro, Rita Belen/N-5442-2014; bonavera, laura/E-9368-2017;
Gonzalez-Nuevo, Joaquin/I-3562-2014; Herranz, Diego/K-9143-2014;
Colombo, Loris/J-2415-2016; Lahteenmaki, Anne/L-5987-2013
OI Barreiro, Rita Belen/0000-0002-6139-4272; bonavera,
laura/0000-0001-8039-3876; Gonzalez-Nuevo, Joaquin/0000-0003-1354-6822;
Herranz, Diego/0000-0003-4540-1417; Colombo, Loris/0000-0003-4572-7732;
FU ESA; CNES (France); CNRS/INSU-IN2P3-INP (France); ASI (Italy); CNR
(Italy); INAF (Italy); NASA (USA); DoE (USA); STFC (UK); UKSA (UK); CSIC
(Spain); MINECO (Spain); JA (Spain); RES (Spain); Tekes (Finland); AoF
(Finland); CSC (Finland); DLR (Germany); MPG (Germany); CSA (Canada);
DTU Space (Denmark); SER/SSO (Switzerland); RCN (Norway); SFI (Ireland);
FCT/MCTES (Portugal); ERC (EU); PRACE (EU); UK BIS NEI grants; Advanced
Computing at IFCA; e-Science team at IFCA
FX The Planck Collaboration acknowledges the support of: ESA; CNES and
CNRS/INSU-IN2P3-INP (France); ASI, CNR, and INAF (Italy); NASA and DoE
(USA); STFC and UKSA (UK); CSIC, MINECO, JA, and RES (Spain); Tekes,
AoF, and CSC (Finland); DLR and MPG (Germany); CSA (Canada); DTU Space
(Denmark); SER/SSO (Switzerland); RCN (Norway); SFI (Ireland); FCT/MCTES
(Portugal); ERC and PRACE (EU). A description of the Planck
Collaboration and a list of its members, indicating which technical or
scientific activities they have been involved in, can be found at
http://www.cosmos.esa.int/web/planck/planck-collaboration. Some of the
results in this paper have been derived using the HEALPix package. We
acknowledge the computer resources, technical expertise and assistance
provided by the Spanish Supercomputing Network (RES) node at Universidad
de Cantabria, and the support provided by the Advanced Computing and
e-Science team at IFCA. Part of this work was undertaken on the STFC
COSMOS@DiRAC HPC Facilities at the University of Cambridge, funded by UK
BIS NEI grants.
NR 118
TC 2
Z9 2
U1 1
U2 1
PU EDP SCIENCES S A
PI LES ULIS CEDEX A
PA 17, AVE DU HOGGAR, PA COURTABOEUF, BP 112, F-91944 LES ULIS CEDEX A,
FRANCE
SN 1432-0746
J9 ASTRON ASTROPHYS
JI Astron. Astrophys.
PD OCT
PY 2016
VL 594
AR A21
DI 10.1051/0004-6361/201525831
PG 30
WC Astronomy & Astrophysics
SC Astronomy & Astrophysics
GA DZ4MG
UT WOS:000385832200014
ER
PT J
AU Ade, PAR
Aghanim, N
Arnaud, M
Arroja, F
Ashdown, M
Aumont, J
Baccigalupi, C
Ballardini, M
Banday, AJ
Barreiro, RB
Bartolo, N
Battaner, E
Benabed, K
Benoit, A
Benoit-Levy, A
Bernard, JP
Bersanelli, M
Bielewicz, P
Bock, JJ
Bonaldi, A
Bonavera, L
Bondi, JR
Borrillu, J
Bouchet, FR
Boulanger, F
Bucher, M
Burigana, C
Butler, RC
Calabrese, E
Cardoso, JF
Catalano, A
Challinor, A
Chamballu, A
Chary, RR
Chiang, HC
Christensen, PR
Churchl, S
Clements, DL
Colombi, S
Colombo, LPL
Combet, C
Contreras, D
Couchot, F
Coulais, A
Crill, BP
Curto, A
Cuttaia, F
Danese, L
Davies, RD
Davis, RJ
de Bernardis, P
de Rosa, A
de Zotti, G
Delabrouillei, J
Desert, FX
Diego, JM
Dole, H
Donzelli, S
Dore, O
Douspis, M
Ducout, A
Dupac, X
Efstathiou, G
Elsner, F
Ensslin, TA
Eriksen, HK
Fergusson, J
Finelli, F
Forni, O
Frailis, M
Fraisse, AA
Franceschi, E
Frejsel, A
Frolov, A
Galeotta, S
Galli, S
Ganga, K
Gauthier, C
Giard, M
Giraud-Heraud, Y
Gjerlow, E
Gonzalez-Nuevo, J
Gorski, KM
Gratton, S
Gregorio, A
Gruppuso, A
Gudmundsson, JE
Hamann, J
Handley, W
Hansen, FK
Hanson, D
Harrison, DL
Henrot-Versille, S
Hernandez-Monteagudo, C
Herranz, D
Hildebrandt, SR
Hivon, E
Hobson, M
Holmes, WA
Hornstrup, A
Hovest, W
Huang, Z
Huffenberger, KM
Hurier, G
Jaffe, AH
Jaffe, TR
Jones, WC
Juvela, M
Keihanen, E
Keskitalo, R
Kim, J
Kisner, TS
Kneissl, R
Knoche, J
Kunz, M
Kurki-Suonio, H
Lagache, G
Lahteenmaki, A
Lamarre, JM
Lasenby, A
Lattanzi, M
Lawrence, CR
Leonardi, R
Lesgourgues, J
Levrier, F
Lewis, A
Liguori, M
Lilje, PB
Linden-Vornle, M
Lopez-Caniego, M
Lubin, PM
Ma, YZ
Macias-Perez, JF
Maggio, G
Maino, D
Mandolesi, N
Mangilli, A
Maris, M
Martini, PG
Martinez-Gonzalez, E
Masi, S
Matarrese, S
McGehee, P
Meinhold, PR
Melchiorri, A
Mendes, L
Mennella, A
Migliaccio, M
Mitra, S
Miville-Deschenes, MA
Molinari, D
Moneti, A
Montier, L
Morgante, G
Mortlock, D
Moss, A
Munchmeyer, M
Munshi, D
Murphy, JA
Naselsky, P
Nati, F
Natoli, P
Netterfield, CB
Norgaard-Nielsen, HU
Noviello, F
Novikov, D
Novikov, I
Oxborrow, CA
Paci, F
Pagano, L
Pajot, F
Paladini, R
Pandolfi, S
Paoletti, D
Pasian, F
Patanchon, G
Pearson, TJ
Peiris, HV
Perdereau, O
Perotto, L
Perrotta, F
Pettorino, V
Piacentini, F
Piat, M
Pierpaoli, E
Pietrobon, D
Plaszczynski, S
Pointecouteau, E
Polenta, G
Popa, L
Pratt, GW
Prezeau, G
Prunet, S
Puget, JL
Rachen, JP
Reach, WT
Rebolo, R
Reinecke, M
Remazeilles, M
Renault, C
Renzi, A
Ristorcelli, I
Rocha, G
Rosset, C
Rossetti, M
Roudier, G
Rowan-Robinson, M
Rubino-Martin, JA
Rusholme, B
Sandri, M
Santos, D
Savelainen, M
Savini, G
Scott, D
Seiffert, MD
Shellard, EPS
Shiraishi, M
Spencer, LD
Stolyarov, V
Stompori, R
Sudiwala, R
Sunyaev, R
Sutton, D
Suur-Uski, AS
Sygnet, JF
Tauber, JA
Terenzi, L
Toffolatti, L
Tomasi, M
Tristram, M
Trombetti, T
Tucci, M
Tuovinen, J
Valenziano, L
Valiviita, J
Van Tent, B
Vielva, P
Villa, F
Wade, LA
Wandelt, BD
Wehus, IK
White, M
Yvon, D
Zacchei, A
Zibin, JP
Zonca, A
AF Ade, P. A. R.
Aghanim, N.
Arnaud, M.
Arroja, F.
Ashdown, M.
Aumont, J.
Baccigalupi, C.
Ballardini, M.
Banday, A. J.
Barreiro, R. B.
Bartolo, N.
Battaner, E.
Benabed, K.
Benoit, A.
Benoit-Levy, A.
Bernard, J. -P.
Bersanelli, M.
Bielewicz, P.
Bock, J. J.
Bonaldi, A.
Bonavera, L.
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Borrillu, J.
Bouchet, F. R.
Boulanger, F.
Bucher, M.
Burigana, C.
Butler, R. C.
Calabrese, E.
Cardoso, J. -F.
Catalano, A.
Challinor, A.
Chamballu, A.
Chary, R. -R.
Chiang, H. C.
Christensen, P. R.
Churchl, S.
Clements, D. L.
Colombi, S.
Colombo, L. P. L.
Combet, C.
Contreras, D.
Couchot, F.
Coulais, A.
Crill, B. P.
Curto, A.
Cuttaia, F.
Danese, L.
Davies, R. D.
Davis, R. J.
de Bernardis, P.
de Rosa, A.
de Zotti, G.
Delabrouillei, J.
Desert, F. -X.
Diego, J. M.
Dole, H.
Donzelli, S.
Dore, O.
Douspis, M.
Ducout, A.
Dupac, X.
Efstathiou, G.
Elsner, F.
Ensslin, T. A.
Eriksen, H. K.
Fergusson, J.
Finelli, F.
Forni, O.
Frailis, M.
Fraisse, A. A.
Franceschi, E.
Frejsel, A.
Frolov, A.
Galeotta, S.
Galli, S.
Ganga, K.
Gauthier, C.
Giard, M.
Giraud-Heraud, Y.
Gjerlow, E.
Gonzalez-Nuevo, J.
Gorski, K. M.
Gratton, S.
Gregorio, A.
Gruppuso, A.
Gudmundsson, J. E.
Hamann, J.
Handley, W.
Hansen, F. K.
Hanson, D.
Harrison, D. L.
Henrot-Versille, S.
Hernandez-Monteagudo, C.
Herranz, D.
Hildebrandt, S. R.
Hivon, E.
Hobson, M.
Holmes, W. A.
Hornstrup, A.
Hovest, W.
Huang, Z.
Huffenberger, K. M.
Hurier, G.
Jaffe, A. H.
Jaffe, T. R.
Jones, W. C.
Juvela, M.
Keihanen, E.
Keskitalo, R.
Kim, J.
Kisner, T. S.
Kneissl, R.
Knoche, J.
Kunz, M.
Kurki-Suonio, H.
Lagache, G.
Lahteenmaki, A.
Lamarre, J. -M.
Lasenby, A.
Lattanzi, M.
Lawrence, C. R.
Leonardi, R.
Lesgourgues, J.
Levrier, F.
Lewis, A.
Liguori, M.
Lilje, P. B.
Linden-Vornle, M.
Lopez-Caniego, M.
Lubin, P. M.
Ma, Y. -Z.
Macias-Perez, J. F.
Maggio, G.
Maino, D.
Mandolesi, N.
Mangilli, A.
Maris, M.
Martini, P. G.
Martinez-Gonzalez, E.
Masi, S.
Matarrese, S.
McGehee, P.
Meinhold, P. R.
Melchiorri, A.
Mendes, L.
Mennella, A.
Migliaccio, M.
Mitra, S.
Miville-Deschenes, M. -A.
Molinari, D.
Moneti, A.
Montier, L.
Morgante, G.
Mortlock, D.
Moss, A.
Munchmeyer, M.
Munshi, D.
Murphy, J. A.
Naselsky, P.
Nati, F.
Natoli, P.
Netterfield, C. B.
Norgaard-Nielsen, H. U.
Noviello, F.
Novikov, D.
Novikov, I.
Oxborrow, C. A.
Paci, F.
Pagano, L.
Pajot, F.
Paladini, R.
Pandolfi, S.
Paoletti, D.
Pasian, F.
Patanchon, G.
Pearson, T. J.
Peiris, H. V.
Perdereau, O.
Perotto, L.
Perrotta, F.
Pettorino, V.
Piacentini, F.
Piat, M.
Pierpaoli, E.
Pietrobon, D.
Plaszczynski, S.
Pointecouteau, E.
Polenta, G.
Popa, L.
Pratt, G. W.
Prezeau, G.
Prunet, S.
Puget, J. -L.
Rachen, J. P.
Reach, W. T.
Rebolo, R.
Reinecke, M.
Remazeilles, M.
Renault, C.
Renzi, A.
Ristorcelli, I.
Rocha, G.
Rosset, C.
Rossetti, M.
Roudier, G.
Rowan-Robinson, M.
Rubino-Martin, J. A.
Rusholme, B.
Sandri, M.
Santos, D.
Savelainen, M.
Savini, G.
Scott, D.
Seiffert, M. D.
Shellard, E. P. S.
Shiraishi, M.
Spencer, L. D.
Stolyarov, V.
Stompori, R.
Sudiwala, R.
Sunyaev, R.
Sutton, D.
Suur-Uski, A. -S.
Sygnet, J. -F.
Tauber, J. A.
Terenzi, L.
Toffolatti, L.
Tomasi, M.
Tristram, M.
Trombetti, T.
Tucci, M.
Tuovinen, J.
Valenziano, L.
Valiviita, J.
Van Tent, B.
Vielva, P.
Villa, F.
Wade, L. A.
Wandelt, B. D.
Wehus, I. K.
White, M.
Yvon, D.
Zacchei, A.
Zibin, J. P.
Zonca, A.
CA Planck Collaboration
TI Planck 2015 results XX. Constraints on inflation
SO ASTRONOMY & ASTROPHYSICS
LA English
DT Article
DE cosmic background radiation; cosmology: theory; early Universe;
inflation
ID PROBE WMAP OBSERVATIONS; MICROWAVE BACKGROUND POLARIZATION; BARYON
ACOUSTIC-OSCILLATIONS; LARGE-SCALE STRUCTURE; PRE-BIG-BANG; COSMOLOGICAL
PERTURBATIONS; TENSOR PERTURBATIONS; EXPANDING UNIVERSE; NATURAL
INFLATION; 2-FIELD INFLATION
AB We present the implications for cosmic inflation of the Planck measurements of the cosmic microwave background (CMB) anisotropies in both temperature and polarization based on the full Planck survey, which includes more than twice the integration time of the nominal survey used for the 2013 release papers. The Planck full mission temperature data and a first release of polarization data on large angular scales measure the spectral index of curvature perturbations to be n(s) = 0.968 +/- 0.006 and tightly constrain its scale dependence to dn(s)/dln k = -0.003 +/- 0.007 when combined with the Planck lensing likelihood. When the Planck high-l polarization data are included, the results are consistent and uncertainties are further reduced. The upper bound on the tensor-to-scalar ratio is r(0).(002) < 0.11 (95% CL). This upper limit is consistent with the B-mode polarization constraint r < 0.12 (95% CL) obtained from a joint analysis of the BICEP2/Keck Array and Planck data. These results imply that V(phi) proportional to phi(2) and natural inflation are now disfavoured compared to models predicting a smaller tensor-to-scalar ratio, such as R-2 inflation. We search for several physically motivated deviations from a simple power-law spectrum of curvature perturbations, including those motivated by a reconstruction of the inflaton potential not relying on the slow-roll approximation. We find that such models are not preferred, either according to a Bayesian model comparison or according to a frequentist simulation-based analysis. Three independent methods reconstructing the primordial power spectrum consistently recover a featureless and smooth P-R (k) over the range of scales 0.008 Mpc(-1) less than or similar to k less than or similar to 0.1 Mpc(-1). At large scales, each method finds deviations from a power law, connected to a deficit at multipoles l approximate to 20-40 in the temperature power spectrum, but at an uncompelling statistical significance owing to the large cosmic variance present at these multipoles. By combining power spectrum and non-Gaussianity bounds, we constrain models with generalized Lagrangians, including Galileon models and axion monodromy models. The Planck data are consistent with adiabatic primordial perturbations, and the estimated values for the parameters of the base Lambda cold dark matter (Lambda CDM) model are not significantly altered when more general initial conditions are admitted. In correlated mixed adiabatic and isocurvature models, the 95% CL upper bound for the non-adiabatic contribution to the observed CMB temperature variance is vertical bar alpha(non-adi)vertical bar < 1.9%, 4.0%, and 2.9% for CDM, neutrino density, and neutrino velocity isocurvature modes, respectively. We have tested inflationary models producing an anisotropic modulation of the primordial curvature power spectrum finding that the dipolar modulation in the CMB temperature field induced by a CDM isocurvature perturbation is not preferred at a statistically significant level. We also establish tight constraints on a possible quadrupolar modulation of the curvature perturbation. These results are consistent with the Planck 2013 analysis based on the nominal mission data and further constrain slow-roll single-field inflationary models, as expected from the increased precision of Planck data using the full set of observations.
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[Arnaud, M.; Chamballu, A.; Pratt, G. W.] Univ Paris Diderot, CEA Saclay, CNRS, Lab AIM,IRFU Serv Astrophys,CEA DSM, Bat 709, F-91191 Gif Sur Yvette, France.
[Cardoso, J. -F.] CNRS, UMR 5141, Lab Traitement & Commun Informat, 46 Rue Barrault, F-75634 Paris 13, France.
[Cardoso, J. -F.] Telecom ParisTech, 46 Rue Barrault, F-75634 Paris 13, France.
[Catalano, A.; Combet, C.; Macias-Perez, J. F.; Perotto, L.; Renault, C.; Santos, D.] Univ Grenoble Alpes, Lab Phys Subat & Cosmol, CNRS IN2P3, 53 Rue Martyrs, F-38026 Grenoble, France.
[Van Tent, B.] Univ Paris Sud 11, Lab Phys Theor, Batiment 210, F-91405 Orsay, France.
[Van Tent, B.] CNRS, Batiment 210, F-91405 Orsay, France.
[Kisner, T. S.] Lawrence Berkeley Natl Lab, Berkeley, CA USA.
[Novikov, D.; Novikov, I.] Russian Acad Sci, Ctr Astro Space, Lebedev Phys Inst, 84-32 Profsoyuznaya St,GSP-7, Moscow 117997, Russia.
[Arroja, F.; Gauthier, C.] Natl Taiwan Univ, Leung Ctr Cosmol & Particle Astrophys, Taipei 10617, Taiwan.
[Ensslin, T. A.; Hernandez-Monteagudo, C.; Hovest, W.; Kim, J.; Knoche, J.; Rachen, J. P.; Reinecke, M.; Sunyaev, R.] Max Planck Inst Astrophys, Karl Schwarzschild Str 1, D-85741 Garching, Germany.
[Hanson, D.] McGill Univ, McGill Phys, Ernest Rutherford Phys Bldg,3600 Rue Univ, Montreal, PQ H3A 2T8, Canada.
[Murphy, J. A.] Natl Univ Ireland, Dept Expt Phys, Maynooth, Kildare, Ireland.
[Bielewicz, P.] Nicolaus Copernicus Astron Ctr, Bartycka 18, PL-00716 Warsaw, Poland.
[Christensen, P. R.; Frejsel, A.; Novikov, I.] Niels Bohr Inst, Blegdamsvej 17, DK-1165 Copenhagen, Denmark.
[Naselsky, P.] Univ Copenhagen, Niels Bohr Inst, Blegdamsvej 17, DK-1165 Copenhagen, Denmark.
[Gudmundsson, J. E.] Nordita Nord Inst Theoret Phys, Roslagstullsbacken 23, S-10691 Stockholm, Sweden.
[Savini, G.] UCL, Opt Sci Lab, Gower St, London, England.
[Baccigalupi, C.; Bielewicz, P.; Danese, L.; de Zotti, G.; Paci, F.; Perrotta, F.] SISSA, Astrophys Sect, Via Bonomea 265, I-34136 Trieste, Italy.
[Terenzi, L.] Univ E Campus, SMARTEST Res Ctr, Via Isimbardi 10, I-22060 Novedrate, CO, Italy.
[Ade, P. A. R.; Benoit, A.; Munshi, D.; Spencer, L. D.] Cardiff Univ, Sch Phys & Astron, Queens Bldg, Cardiff CF24 3AA, S Glam, Wales.
[Moss, A.] Univ Nottingham, Sch Phys & Astron, Nottingham NG7 2RD, England.
[Frolov, A.] Simon Fraser Univ, Dept Phys, 8888 Univ Dr, Burnaby, BC, Canada.
[Bouchet, F. R.] Sorbonne Univ UPMC, UMR 7095, Inst Astrophys Paris, 98bis Blvd Arago, F-75014 Paris, France.
[Sunyaev, R.] Russian Acad Sci, Space Res Inst IKI, Profsoyuznaya Str 84-32, Moscow 117997, Russia.
[Borrillu, J.] Univ Calif Berkeley, Space Sci Lab, Berkeley, CA 94720 USA.
[Stolyarov, V.] Russian Acad Sci, Special Astrophys Observ, Karachai Cherkessian Rep, Zelenchukskiy R, Russia.
[Churchl, S.] Stanford Univ, Dept Phys, Varian Phys Bldg,382 Via Pueblo Mall, Stanford, CA USA.
[Calabrese, E.] Univ Oxford, Subdept Astrophys, Keble Rd, Oxford OX1 3RH, England.
[Hamann, J.] Univ Sydney, Sch Phys A28, Sydney Inst Astron, Sydney, NSW 2006, Australia.
[Gudmundsson, J. E.] Stockholm Univ, Dept Phys, Oskar Klein Ctr Cosmoparticle Phys, AlbaNova, S-10691 Stockholm, Sweden.
[Hamann, J.; Lesgourgues, J.] CERN, PH TH, Div Theory, CH-1211 Geneva 23, Switzerland.
[Benabed, K.; Benoit-Levy, A.; Colombi, S.; Elsner, F.; Hivon, E.; Prunet, S.; Wandelt, B. D.] UPMC Univ Paris 06, UMR7095, 98bis Blvd Arago, F-75014 Paris, France.
[Banday, A. J.; Bernard, J. -P.; Forni, O.; Giard, M.; Jaffe, T. R.; Montier, L.; Pointecouteau, E.; Ristorcelli, I.] Univ Toulouse, UPS OMP, IRAP, F-31028 Toulouse 4, France.
[Reach, W. T.] Univ Space Res Assoc, Stratospher Observ Infrared Astron, MS 232-11, Moffett Field, CA 94035 USA.
[Battaner, E.] Univ Granada, Dept Fis Teor & Cosmos, Fac Ciencias, E-18071 Granada, Spain.
[Battaner, E.] Univ Granada, Inst Carlos Fis Teor & Computac 1, Granada 18071, Spain.
[Gorski, K. M.] Univ Warsaw Observ, Aleje Ujazdowskie 4, PL-00478 Warsaw, Poland.
RP Bucher, M (reprint author), Univ Paris Diderot, APC, CNRS IN2P3, CEA Lrfu,Observ Paris,Sorbonne Paris Cite, 10 Rue Alice Domon & Leonie Duquet, F-75205 Paris 13, France.; Finelli, F (reprint author), INAF IASF Bologna, Via Gobetti 101, I-40127 Bologna, Italy.; Finelli, F (reprint author), Ist Nazl Fis Nucl, Sez Bologna, Via Irnerio 46, I-40126 Bologna, Italy.
EM bucher@apc.univ-paris7.fr; finelli@iasfbo.inaf.it
RI Lahteenmaki, Anne/L-5987-2013; Barreiro, Rita Belen/N-5442-2014;
bonavera, laura/E-9368-2017; Gonzalez-Nuevo, Joaquin/I-3562-2014;
Herranz, Diego/K-9143-2014; Colombo, Loris/J-2415-2016;
OI Juvela, Mika/0000-0002-5809-4834; Valiviita, Jussi/0000-0001-6225-3693;
Huang, Zhiqi/0000-0002-1506-1063; Kurki-Suonio,
Hannu/0000-0002-4618-3063; Molinari, Diego/0000-0002-7799-3915; Zacchei,
Andrea/0000-0003-0396-1192; Toffolatti, Luigi/0000-0003-2645-7386;
Lilje, Per/0000-0003-4324-7794; Nati, Federico/0000-0002-8307-5088;
Savini, Giorgio/0000-0003-4449-9416; Pierpaoli,
Elena/0000-0002-7957-8993; Barreiro, Rita Belen/0000-0002-6139-4272;
bonavera, laura/0000-0001-8039-3876; Gonzalez-Nuevo,
Joaquin/0000-0003-1354-6822; Herranz, Diego/0000-0003-4540-1417;
Colombo, Loris/0000-0003-4572-7732; Hivon, Eric/0000-0003-1880-2733;
Paoletti, Daniela/0000-0003-4761-6147; TERENZI,
LUCA/0000-0001-9915-6379; Stolyarov, Vladislav/0000-0001-8151-828X;
Reach, William/0000-0001-8362-4094
FU ESA; CNES (France); CNRS/INSU-IN2P3-INP (France); ASI (Italy); CNR
(Italy); INAF (Italy); NASA (USA); DoE (USA); STFC (UK); UKSA (UK); CSIC
(Spain); MINECO (Spain); JA (Spain); RES (Spain); Tekes (Finland); AoF
(Finland); CSC (Finland); DLR (Germany); MPG (Germany); CSA (Canada);
DTU Space (Denmark); SER/SSO (Switzerland); RCN (Norway); SFI (Ireland);
FCT/MCTES (Portugal); ERC (EU); PRACE (EU); Office of Science of the US
Department of Energy [DE-AC02-05CH11231]; UK BIS National
E-infrastructure capital grants
FX The Planck Collaboration acknowledges the support of: ESA; CNES and
CNRS/INSU-IN2P3-INP (France); ASI, CNR, and INAF (Italy); NASA and DoE
(USA); STFC and UKSA (UK); CSIC, MINECO, JA, and RES (Spain); Tekes,
AoF, and CSC (Finland); DLR and MPG (Germany); CSA (Canada); DTU Space
(Denmark); SER/SSO (Switzerland); RCN (Norway); SFI (Ireland); FCT/MCTES
(Portugal); ERC and PRACE (EU). A description of the Planck
Collaboration and a list of its members, indicating which technical or
scientific activities they have been involved in, can be found at
http://www.cosmos.esa.int/web/planck/planck-collaboration. This research
used resources of the National Energy Research Scientific Computing
Center, a DOE Office of Science User Facility supported by the Office of
Science of the US Department of Energy under Contract No.
DE-AC02-05CH11231. Part of this work was undertaken at the STFC DiRAC
HPC Facilities at the University of Cambridge, funded by UK BIS National
E-infrastructure capital grants. We gratefully acknowledge the IN2P3
Computer Center (http://cc.in2p3.fr) for providing a significant amount
of the computing resources and services needed for this work.
NR 280
TC 68
Z9 68
U1 3
U2 3
PU EDP SCIENCES S A
PI LES ULIS CEDEX A
PA 17, AVE DU HOGGAR, PA COURTABOEUF, BP 112, F-91944 LES ULIS CEDEX A,
FRANCE
SN 1432-0746
J9 ASTRON ASTROPHYS
JI Astron. Astrophys.
PD OCT
PY 2016
VL 594
AR A20
DI 10.1051/0004-6361/201525898
PG 65
WC Astronomy & Astrophysics
SC Astronomy & Astrophysics
GA DZ4MG
UT WOS:000385832200018
ER
PT J
AU Ade, PAR
Aghanim, N
Arnaud, M
Arrojam, F
Ashdown, M
Aumont, J
Baccigalupi, C
Ballardini, M
Banday, AJ
Barreiro, RB
Bartolo, N
Basak, S
Battaner, E
Benabed, K
Benoit, A
Benoit-Levy, A
Bernard, JP
Bersanelli, M
Bielewicz, P
Bock, JJ
Bonaldi, A
Bonavera, L
Bond, JR
Borrill, J
Bouchet, FR
Boulanger, F
Bucher, M
Burigana, C
Butler, RC
Calabrese, E
Cardoso, JF
Catalano, A
Challinor, A
Chamballu, A
Chiang, HC
Christensen, PR
Church, S
Clements, DL
Colombi, S
Colombo, LPL
Combet, C
Couchot, F
Coulais, A
Crill, BP
Curto, A
Cuttaia, F
Danese, L
Davies, RD
Davis, RJ
de Bernardis, P
de Rosa, A
de Zotti, G
Delabrouille, J
Desert, FX
Diego, JM
Dole, H
Donzelli, S
Dore, O
Douspis, M
Ducout, A
Dupac, X
Efstathiou, G
Elsner, F
Ensslin, TA
Eriksen, HK
Fergusson, J
Finelli, F
Forni, O
Frailis, M
Fraisse, AA
Franceschi, E
Frejsel, A
Galeotta, S
Galli, S
Ganga, K
Gauthier, C
Ghosh, T
Giard, M
Giraud-Heraud, Y
Gjerlow, E
Gonzalez-Nuevo, J
Gorski, KM
Gratton, S
Gregorio, A
Gruppuso, A
Gudmundsson, JE
Hamann, J
Hansen, FK
Hanson, D
Harrison, DL
Heavens, A
Helou, G
Henrot-Versille, S
Hernandez-Monteagudo, C
Herranz, D
Hildebrandt, SR
Hivon, E
Hobson, M
Holmes, WA
Hornstrup, A
Hovest, W
Huang, Z
Huffenberger, KM
Hurier, G
Jaffe, AH
Jaffe, TR
Jones, WC
Juvela, M
Keihanen, E
Keskitalo, R
Kim, J
Kisner, TS
Knoche, J
Kunz, M
Kurki-Suonio, H
Lacasa, F
Lagache, G
Lahteenmaki, A
Lamarre, JM
Lasenby, A
Lattanzi, M
Lawrence, CR
Leonardi, R
Lesgourgues, J
Levrier, F
Lewis, A
Liguori, M
Lilje, PB
Linden-Vornle, M
Lopez-Caniego, M
Lubin, PM
Macias-Perez, JF
Maggio, G
Maino, D
Mandolesi, N
Mangilli, A
Marinucci, D
Maris, M
Martin, PG
Martinez-Gonzalez, E
Masi, S
Matarrese, S
McGehee, P
Meinhold, PR
Melchiorri, A
Mendes, L
Mennella, A
Migliaccio, M
Mitra, S
Miville-Deschenes, MA
Moneti, A
Montier, L
Morgante, G
Mortlock, D
Moss, A
Munchmeyer, M
Munshi, D
Murphy, JA
Naselsky, P
Nati, F
Natoli, P
Netterfield, CB
Norgaard-Nielsen, HU
Noviello, F
Novikov, D
Novikov, I
Oxborrow, CA
Paci, F
Pagano, L
Pajot, F
Paoletti, D
Pasian, F
Patanchon, G
Peiris, HV
Perdereau, O
Perotto, L
Perrotta, F
Pettorino, V
Piacentini, F
Piat, M
Pierpaoli, E
Pietrobon, D
Plaszczynski, S
Pointecouteau, E
Polenta, G
Popa, L
Pratt, GW
Prezeau, G
Prunet, S
Puget, JL
Rachen, JP
Racine, B
Rebolo, R
Reinecke, M
Remazeilles, M
Renault, C
Renzi, A
Ristorcelli, I
Rocha, G
Rosset, C
Rossetti, M
Roudier, G
Rubino-Martin, JA
Rusholme, B
Sandri, M
Santos, D
Savelainen, M
Savini, G
Scott, D
Seiffert, MD
Shellard, EPS
Shiraishi, M
Smith, K
Spencer, LD
Stolyarov, V
Stompor, R
Sudiwala, R
Sunyaev, R
Sutter, P
Sutton, D
Suur-Uski, AS
Sygnet, JF
Tauber, JA
Terenzi, L
Toffolatti, L
Tomasi, M
Tristram, M
Troja, A
Tucci, M
Tuovinen, J
Valenziano, L
Valiyiita, J
Van Tent, B
Vielva, P
Villas, F
Wade, LA
Wandelt, BD
Wehus, IK
Yvon, D
Zacchei, A
Zonca, A
AF Ade, P. A. R.
Aghanim, N.
Arnaud, M.
Arrojam, F.
Ashdown, M.
Aumont, J.
Baccigalupi, C.
Ballardini, M.
Banday, A. J.
Barreiro, R. B.
Bartolo, N.
Basak, S.
Battaner, E.
Benabed, K.
Benoit, A.
Benoit-Levy, A.
Bernard, J. -P.
Bersanelli, M.
Bielewicz, P.
Bock, J. J.
Bonaldi, A.
Bonavera, L.
Bond, J. R.
Borrill, J.
Bouchet, F. R.
Boulanger, F.
Bucher, M.
Burigana, C.
Butler, R. C.
Calabrese, E.
Cardoso, J. -F.
Catalano, A.
Challinor, A.
Chamballu, A.
Chiang, H. C.
Christensen, P. R.
Church, S.
Clements, D. L.
Colombi, S.
Colombo, L. P. L.
Combet, C.
Couchot, F.
Coulais, A.
Crill, B. P.
Curto, A.
Cuttaia, F.
Danese, L.
Davies, R. D.
Davis, R. J.
de Bernardis, P.
de Rosa, A.
de Zotti, G.
Delabrouille, J.
Desert, F. -X.
Diego, J. M.
Dole, H.
Donzelli, S.
Dore, O.
Douspis, M.
Ducout, A.
Dupac, X.
Efstathiou, G.
Elsner, F.
Ensslin, T. A.
Eriksen, H. K.
Fergusson, J.
Finelli, F.
Forni, O.
Frailis, M.
Fraisse, A. A.
Franceschi, E.
Frejsel, A.
Galeotta, S.
Galli, S.
Ganga, K.
Gauthier, C.
Ghosh, T.
Giard, M.
Giraud-Heraud, Y.
Gjerlow, E.
Gonzalez-Nuevo, J.
Gorski, K. M.
Gratton, S.
Gregorio, A.
Gruppuso, A.
Gudmundsson, J. E.
Hamann, J.
Hansen, F. K.
Hanson, D.
Harrison, D. L.
Heavens, A.
Helou, G.
Henrot-Versille, S.
Hernandez-Monteagudo, C.
Herranz, D.
Hildebrandt, S. R.
Hivon, E.
Hobson, M.
Holmes, W. A.
Hornstrup, A.
Hovest, W.
Huang, Z.
Huffenberger, K. M.
Hurier, G.
Jaffe, A. H.
Jaffe, T. R.
Jones, W. C.
Juvela, M.
Keihanen, E.
Keskitalo, R.
Kim, J.
Kisner, T. S.
Knoche, J.
Kunz, M.
Kurki-Suonio, H.
Lacasa, F.
Lagache, G.
Lahteenmaki, A.
Lamarre, J. -M.
Lasenby, A.
Lattanzi, M.
Lawrence, C. R.
Leonardi, R.
Lesgourgues, J.
Levrier, F.
Lewis, A.
Liguori, M.
Lilje, P. B.
Linden-Vornle, M.
Lopez-Caniego, M.
Lubin, P. M.
Macias-Perez, J. F.
Maggio, G.
Maino, D.
Mandolesi, N.
Mangilli, A.
Marinucci, D.
Maris, M.
Martin, P. G.
Martinez-Gonzalez, E.
Masi, S.
Matarrese, S.
McGehee, P.
Meinhold, P. R.
Melchiorri, A.
Mendes, L.
Mennella, A.
Migliaccio, M.
Mitra, S.
Miville-Deschenes, M. -A.
Moneti, A.
Montier, L.
Morgante, G.
Mortlock, D.
Moss, A.
Munchmeyer, M.
Munshi, D.
Murphy, J. A.
Naselsky, P.
Nati, F.
Natoli, P.
Netterfield, C. B.
Norgaard-Nielsen, H. U.
Noviello, F.
Novikov, D.
Novikov, I.
Oxborrow, C. A.
Paci, F.
Pagano, L.
Pajot, F.
Paoletti, D.
Pasian, F.
Patanchon, G.
Peiris, H. V.
Perdereau, O.
Perotto, L.
Perrotta, F.
Pettorino, V.
Piacentini, F.
Piat, M.
Pierpaoli, E.
Pietrobon, D.
Plaszczynski, S.
Pointecouteau, E.
Polenta, G.
Popa, L.
Pratt, G. W.
Prezeau, G.
Prunet, S.
Puget, J. -L.
Rachen, J. P.
Racine, B.
Rebolo, R.
Reinecke, M.
Remazeilles, M.
Renault, C.
Renzi, A.
Ristorcelli, I.
Rocha, G.
Rosset, C.
Rossetti, M.
Roudier, G.
Rubino-Martin, J. A.
Rusholme, B.
Sandri, M.
Santos, D.
Savelainen, M.
Savini, G.
Scott, D.
Seiffert, M. D.
Shellard, E. P. S.
Shiraishi, M.
Smith, K.
Spencer, L. D.
Stolyarov, V.
Stompor, R.
Sudiwala, R.
Sunyaev, R.
Sutter, P.
Sutton, D.
Suur-Uski, A. -S.
Sygnet, J. -F.
Tauber, J. A.
Terenzi, L.
Toffolatti, L.
Tomasi, M.
Tristram, M.
Troja, A.
Tucci, M.
Tuovinen, J.
Valenziano, L.
Valiyiita, J.
Van Tent, B.
Vielva, P.
Villas, F.
Wade, L. A.
Wandelt, B. D.
Wehus, I. K.
Yvon, D.
Zacchei, A.
Zonca, A.
CA Planck Collaboration
TI Planck 2015 results XVII. Constraints on primordial non-Gaussianity
SO ASTRONOMY & ASTROPHYSICS
LA English
DT Article
DE cosmic background radiation; cosmology: observations; cosmology: theory;
early Universe; inflation; methods: data analysis
ID MICROWAVE BACKGROUND BISPECTRUM; LARGE-SCALE STRUCTURE; 3-POINT
CORRELATION-FUNCTION; PROBE WMAP OBSERVATIONS; MINKOWSKI FUNCTIONALS;
POLARIZATION ANISOTROPIES; PARAMETER F(NL); FAST ESTIMATOR; POINT
SOURCES; INFLATION
AB The Planck full mission cosmic microwave background (CMB) temperature and E-mode polarization maps are analysed to obtain constraints on primordial non-Gaussianity (NG). Using three classes of optimal bispectrum estimators - separable template-fitting (KSW), binned, and modal we obtain consistent values for the primordial local, equilateral, and orthogonal bispectrum amplitudes, quoting as our final result from temperature alone f(NL)(local) = 2.5 +/- 5.7, f(NL)(equil) = 16 +/- 70, and f(NL)(ortho) = 34 +/- 33 (68% CL, statistical). Combining temperature and polarization data we obtain f(NL)(local) = 0.8 +/- 5.0, f(NL)(equil) = 4 +/- 43, and f(NL)(ortho) = 26 +/- 21 (68% CL, statistical). The results are based on comprehensive cross-validation of these estimators on Gaussian and non-Gaussian simulations, are stable across component separation techniques, pass an extensive suite of tests, and are consistent with estimators based on measuring the Minkowski functionals of the CMB. The effect of time-domain de-glitching systematics on the bispectrum is negligible. In spite of these test outcomes we conservatively label the results including polarization data as preliminary, owing to a known mismatch of the noise model in simulations and the data. Beyond estimates of individual shape amplitudes, we present model-independent, three-dimensional reconstructions of the Planck CMB bispectrum and derive constraints on early universe scenarios that generate primordial NG, including general single-field models of inflation, axion inflation, initial state modifications, models producing parity-violating tensor bispectra, and directionally dependent vector models. We present a wide survey of scale-dependent feature and resonance models, accounting for the "look elsewhere" effect in estimating the statistical significance of features. We also look for isocurvature NG, and find no signal, but we obtain constraints that improve significantly with the inclusion of polarization. The primordial trispectrum amplitude in the local model is constrained to be g(NL)(local) = (9.0 +/- 7.7) x 10(4) (68% CL statistical), and we perform an analysis of trispectrum shapes beyond the local case. The global picture that emerges is one of consistency with the premises of the Lambda CDM cosmology, namely that the structure we observe today was sourced by adiabatic, passive, Gaussian, and primordial seed perturbations.
C1 [Bucher, M.; Cardoso, J. -F.; Delabrouille, J.; Ganga, K.; Gauthier, C.; Giraud-Heraud, Y.; Patanchon, G.; Piat, M.; Racine, B.; Remazeilles, M.; Rosset, C.; Roudier, G.; Stompor, R.] Univ Paris Diderot, APC, CNRS IN2P3, CEA Lrfu,Observ Paris,Sorbonne Paris Cite, 10 Rue Alice Domon & Leonie Duquet, F-75205 Paris 13, France.
[Lahteenmaki, A.] Aalto Univ, Metsahovi Radio Observ, POB 13000, Aalto 00076, Finland.
[Lahteenmaki, A.] Aalto Univ, Dept Radio Sci & Engn, POB 13000, Aalto 00076, Finland.
[Kunz, M.] African Inst Math Sci, 6-8 Melrose Rd, ZA-7945 Cape Town, South Africa.
[Natoli, P.; Polenta, G.] Agenzia Spaziale Italiana, Sci Data Ctr, Via Politecn Snc, I-00133 Rome, Italy.
[Lagache, G.] Aix Marseille Univ, CNRS, LAM, F-13388 Marseille, France.
[Ashdown, M.; Curto, A.; Hobson, M.; Lasenby, A.; Stolyarov, V.] Univ Cambridge, Cavendish Lab, Astrophys Grp, JJ Thomson Ave, Cambridge CB3 0HE, England.
[Chiang, H. C.] Univ KwaZulu Natal, Sch Math Stat & Comp Sci, Astrophys & Cosmol Res Unit, Westville Campus,Private Bag X54001, ZA-4000 Durban, South Africa.
[Leonardi, R.] CGEE, SCS Qd 9,Lote C,Torre C,4 Andar, BR-70308200 Brasilia, DF, Brazil.
[Bond, J. R.; Hanson, D.; Huang, Z.; Martin, P. G.; Miville-Deschenes, M. -A.] Univ Toronto, CITA, 60 St George St, Toronto, ON M5S 3H8, Canada.
[Banday, A. J.; Bernard, J. -P.; Bielewicz, P.; Forni, O.; Giard, M.; Jaffe, T. R.; Montier, L.; Pointecouteau, E.; Ristorcelli, I.] IRAP, CNRS, 9 Ave Colonel Roche,BP 44346, F-31028 Toulouse 4, France.
[Tuovinen, J.] Trinity Coll Dublin, CRANN, Dublin, Ireland.
[Bock, J. J.; Crill, B. P.; Dore, O.; Helou, G.; Hildebrandt, S. R.; Prezeau, G.; Rocha, G.; Seiffert, M. D.] CALTECH, Pasadena, CA 91125 USA.
[Challinor, A.; Fergusson, J.; Shellard, E. P. S.] Univ Cambridge, DAMTP, Ctr Theoret Cosmol, Wilberforce Rd, Cambridge CB3 0WA, England.
[Hernandez-Monteagudo, C.] CEFCA, Plaza San Juan,1,Planta 2, Teruel 44001, Spain.
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[Christensen, P. R.] Niels Bohr Inst, Discovery Ctr, Blegdamsvej 17, DK-2100 Copenhagen, Denmark.
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[Rebolo, R.; Rubino-Martin, J. A.] Inst Astrofis Canarias, C Via Lactea S-N, Tenerife 38205, Spain.
[Barreiro, R. B.; Bonavera, L.; Curto, A.; Diego, J. M.; Gonzalez-Nuevo, J.; Herranz, D.; Lopez-Caniego, M.; Martinez-Gonzalez, E.; Vielva, P.] Univ Cantabria, CSIC, Inst Fis Cantabria, Avda Castros S-N, E-39005 Santander, Spain.
[Arrojam, F.; Bartolo, N.; Liguori, M.; Matarrese, S.; Shiraishi, M.] Ist Nazl Fis Nucl, Sez Padova, Via Marzolo 8, I-35131 Padua, Italy.
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[Galli, S.] Univ Chicago, Kavli Inst Cosmol Phys, Chicago, IL 60637 USA.
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[Catalano, A.; Coulais, A.; Lamarre, J. -M.; Levrier, F.; Roudier, G.] Observ Paris, CNRS, LERMA, 61 Ave Observ0, F-75014 Paris, France.
[Arnaud, M.; Chamballu, A.; Pratt, G. W.] Univ Paris Diderot, CEA Saclay, CEA DSM, Lab AIM,IRFU Serv Astrophys,CNRS, Bat 709, F-91191 Gif Sur Yvette, France.
[Cardoso, J. -F.] CNRS, Lab Traitement & Commun Informat, UMR 5141, 46 Rue Barrault, F-75634 Paris 13, France.
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[Van Tent, B.] Univ Paris Sud 11, Lab Phys Theor, Batiment 210, F-91405 Orsay, France.
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[Bielewicz, P.] Nicolaus Copernicus Astron Ctr, Bartycka 18, PL-00716 Warsaw, Poland.
[Christensen, P. R.; Frejsel, A.; Novikov, I.] Niels Bohr Inst, Blegdamsvej 17, DK-2100 Copenhagen, Denmark.
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[Gudmundsson, J. E.] Nordita Nord Inst Theoret Phys, Roslagstullsbacken 23, S-10691 Stockholm, Sweden.
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[Banday, A. J.; Bernard, J. -P.; Forni, O.; Giard, M.; Jaffe, T. R.; Montier, L.; Pointecouteau, E.; Ristorcelli, I.] Univ Toulouse, UPS OMP, IRAP, F-31028 Toulouse 4, France.
[Battaner, E.] Univ Granada, Fac Ciencias, Dept Fis Teor & Cosmos, E-18071 Granada, Spain.
[Battaner, E.] Univ Granada, Inst Carlos Fis Teor & Computac 18071, E-18071 Granada, Spain.
[Gorski, K. M.] Univ Warsaw Observ, Aleje Ujazdowskie 4, PL-00478 Warsaw, Poland.
RP Bartolo, N (reprint author), Univ Padua, Dipartimento Fis & Astron G Galilei, Via Marzolo 8, I-35131 Padua, Italy.; Bartolo, N (reprint author), Ist Nazl Fis Nucl, Sez Padova, Via Marzolo 8, I-35131 Padua, Italy.
EM bartolo@pd.infn.it
RI Lahteenmaki, Anne/L-5987-2013; Barreiro, Rita Belen/N-5442-2014;
bonavera, laura/E-9368-2017; Gonzalez-Nuevo, Joaquin/I-3562-2014;
Herranz, Diego/K-9143-2014; Colombo, Loris/J-2415-2016;
OI Zacchei, Andrea/0000-0003-0396-1192; Toffolatti,
Luigi/0000-0003-2645-7386; Lilje, Per/0000-0003-4324-7794; Paoletti,
Daniela/0000-0003-4761-6147; Nati, Federico/0000-0002-8307-5088; Savini,
Giorgio/0000-0003-4449-9416; Pierpaoli, Elena/0000-0002-7957-8993;
Juvela, Mika/0000-0002-5809-4834; Huang, Zhiqi/0000-0002-1506-1063;
Kurki-Suonio, Hannu/0000-0002-4618-3063; Barreiro, Rita
Belen/0000-0002-6139-4272; bonavera, laura/0000-0001-8039-3876;
Gonzalez-Nuevo, Joaquin/0000-0003-1354-6822; Herranz,
Diego/0000-0003-4540-1417; Colombo, Loris/0000-0003-4572-7732; TERENZI,
LUCA/0000-0001-9915-6379; Stolyarov, Vladislav/0000-0001-8151-828X;
Valiviita, Jussi/0000-0001-6225-3693
FU ESA; CNES (France); CNRS/INSU-IN2P3-INP (France); ASI (Italy); CNR
(Italy); INAF (Italy); NASA (USA); DoE (USA); STFC (UK); UKSA (UK); CSIC
(Spain); MINECO (Spain); JA (Spain); RES (Spain); Tekes (Finland); AoF
(Finland); CSC (Finland); DLR (Germany); MPG (Germany); CSA (Canada);
DTU Space (Denmark); SER/SSO (Switzerland); RCN (Norway); SFI (Ireland);
FCT/MCTES (Portugal); ERC (EU); PRACE (EU); UK BIS NEI grants; Office of
Science of the U.S. Department of Energy [DE-AC02-05CH11231]; Canada
Foundation for Innovation under Compute Canada; Government of Ontario;
University of Toronto
FX The Planck Collaboration acknowledges the support of: ESA; CNES and
CNRS/INSU-IN2P3-INP (France); ASI, CNR, and INAF (Italy); NASA and DoE
(USA); STFC and UKSA (UK); CSIC, MINECO, JA, and RES (Spain); Tekes,
AoF, and CSC (Finland); DLR and MPG (Germany); CSA (Canada); DTU Space
(Denmark); SER/SSO (Switzerland); RCN (Norway); SFI (Ireland); FCT/MCTES
(Portugal); ERC and PRACE (EU). A description of the Planck
Collaboration and a list of its members, indicating which technical or
scientific activities they have been involved in, can be found at
http://www.cosmos.esa.int/web/planck/planck-collaboration. Some of the
results in this paper have been derived using the HEALPix package. Part
of this work was undertaken on the STFC COSMOS@DiRAC HPC Facility at the
University of Cambridge, funded by UK BIS NEI grants. We gratefully
acknowledge IN2P3 Computer Center (http://cc.in2p3.fr) for providing a
significant amount of the computing resources and services needed for
the analysis with the binned bispectrum estimator. This research used
resources of the National Energy Research Scientific Computing Center, a
DOE Office of Science User Facility supported by the Office of Science
of the U.S. Department of Energy under Contract No. DE-AC02-05CH11231.
We also acknowledge the IAP magique3 computer facilities. Some
computations were performed on the GPC cluster at the SciNet HPC
Consortium. SciNet is funded by the Canada Foundation for Innovation
under the auspices of Compute Canada, the Government of Ontario, and the
University of Toronto.
NR 261
TC 17
Z9 17
U1 2
U2 2
PU EDP SCIENCES S A
PI LES ULIS CEDEX A
PA 17, AVE DU HOGGAR, PA COURTABOEUF, BP 112, F-91944 LES ULIS CEDEX A,
FRANCE
SN 1432-0746
J9 ASTRON ASTROPHYS
JI Astron. Astrophys.
PD OCT
PY 2016
VL 594
AR A17
DI 10.1051/0004-6361/201525836
PG 66
WC Astronomy & Astrophysics
SC Astronomy & Astrophysics
GA DZ4MG
UT WOS:000385832200016
ER
PT J
AU Ade, PAR
Aghanim, N
Arnaud, M
Ashdown, M
Aumont, J
Baccigalupi, C
Banday, AJ
Barreiro, RB
Bartlett, JG
Bartolo, N
Battaner, E
Battye, R
Benabed, K
Benoit, A
Benoit-Levy, A
Bernard, JP
Bersanelli, M
Bielewicz, P
Bock, JJ
Bonaldi, A
Bonavera, L
Bond, JR
Borrill, J
Bouchet, FR
Boulanger, F
Bucher, M
Burigana, C
Butler, RC
Calabrese, E
Cardoso, JF
Catalano, A
Challinor, A
Chamballu, A
Chary, RR
Chiang, HC
Chluba, J
Christensen, PR
Church, S
Clements, DL
Colombi, S
Colombo, LPL
Combet, C
Coulais, A
Crill, BP
Curto, A
Cuttaia, F
Danese, L
Davies, RD
Davis, RJ
de Bernardis, P
de Rosa, A
de Zotti, G
Delabrouille, J
Desert, FX
Di Valentino, E
Dickinson, C
Diego, JM
Dolag, K
Dole, H
Donzelli, S
Dore, O
Douspis, M
Ducout, A
Dunkley, J
Dupac, X
Efstathiou, G
Elsner, F
Ensslin, TA
Eriksen, HK
Farhang, M
Fergusson, J
Finelli, F
Forni, O
Frailis, M
Fraisse, AA
Franceschi, E
Frejsel, A
Galeotta, S
Galli, S
Ganga, K
Gauthier, C
Gerbino, M
Ghosh, T
Giard, M
Giraud-Heraud, Y
Giusarma, E
Gjerlow, E
Gonzalez-Nuevo, J
Gorski, KM
Gratton, S
Gregorio, A
Gruppuso, A
Gudmundsson, JE
Hamann, J
Hansen, FK
Hanson, D
Harrison, DL
Helou, G
Henrot-Versille, S
Hernandez-Monteagudo, C
Herranz, D
Hildebrandt, SR
Hivon, E
Hobson, M
Holmes, WA
Hornstrup, A
Hovest, W
Huang, Z
Huffenberger, KM
Hurier, G
Jaffe, AH
Jaffe, TR
Jones, WC
Juvela, M
Keihanen, E
Keskitalo, R
Kisner, TS
Kneissl, R
Knoche, J
Knox, L
Kunz, M
Kurki-Suonio, H
Lagache, G
Lahteenmaki, A
Lamarre, JM
Lasenby, A
Lattanzi, M
Lawrence, CR
Leahy, JP
Leonardi, R
Lesgourgues, J
Levrier, F
Lewis, A
Liguori, M
Lilje, PB
Linden-Vornle, M
Lopez-Caniego, M
Lubin, PM
Macias-Perez, JF
Maggio, G
Maino, D
Mandolesi, N
Mangilli, A
Marchini, A
Maris, M
Martin, PG
Martinelli, M
Martinez-Gonzalez, E
Masi, S
Matarrese, S
McGehee, P
Meinhold, PR
Melchiorri, A
Melin, JB
Mendes, L
Mennella, A
Migliaccio, M
Millea, M
Mitra, S
Miville-Deschenes, MA
Moneti, A
Montier, L
Morgante, G
Mortlock, D
Moss, A
Munshi, D
Murphy, JA
Naselsky, P
Nati, F
Natoli, P
Netterfield, CB
Norgaard-Nielsen, HU
Noviello, F
Novikov, D
Novikov, I
Oxborrow, CA
Paci, F
Pagano, L
Pajot, F
Paladini, R
Paoletti, D
Partridge, B
Pasian, F
Patanchon, G
Pearson, TJ
Perdereau, O
Perotto, L
Perrotta, F
Pettorino, V
Piacentini, F
Piat, M
Pierpaoli, E
Pietrobon, D
Plaszczynski, S
Pointecouteau, E
Polenta, G
Popa, L
Pratt, GW
Prezeau, G
Prunet, S
Puget, JL
Rachen, JP
Reach, WT
Rebolo, R
Reinecke, M
Remazeilles, M
Renault, C
Renzi, A
Ristorcelli, I
Rocha, G
Rosset, C
Rossetti, M
Roudier, G
d'Orfeui, BR
Rowan-Robinson, M
Rubino-Martin, JA
Rusholme, B
Said, N
Salvatelli, V
Salvati, L
Sandri, M
Santos, D
Savelainen, M
Savini, G
Scott, D
Seiffert, MD
Serra, P
Shellard, EPS
Spencer, LD
Spinelli, M
Stolyarov, V
Stompor, R
Sudiwala, R
Sunyaev, R
Sutton, D
Suur-Uski, AS
Sygnet, JF
Tauber, JA
Terenzi, L
Toffolatti, L
Tomasi, M
Tristram, M
Trombetti, T
Tucci, M
Tuovinen, J
Turler, M
Umana, G
Valenziano, L
Valiviita, J
Van Tent, F
Vielva, P
Villa, F
Wade, LA
Wandelt, BD
Wehus, IK
White, M
White, SDM
Wilkinson, A
Yvon, D
Zacchei, A
Zonca, A
AF Ade, P. A. R.
Aghanim, N.
Arnaud, M.
Ashdown, M.
Aumont, J.
Baccigalupi, C.
Banday, A. J.
Barreiro, R. B.
Bartlett, J. G.
Bartolo, N.
Battaner, E.
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de Rosa, A.
de Zotti, G.
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Desert, F. -X.
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Dickinson, C.
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Dole, H.
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Franceschi, E.
Frejsel, A.
Galeotta, S.
Galli, S.
Ganga, K.
Gauthier, C.
Gerbino, M.
Ghosh, T.
Giard, M.
Giraud-Heraud, Y.
Giusarma, E.
Gjerlow, E.
Gonzalez-Nuevo, J.
Gorski, K. M.
Gratton, S.
Gregorio, A.
Gruppuso, A.
Gudmundsson, J. E.
Hamann, J.
Hansen, F. K.
Hanson, D.
Harrison, D. L.
Helou, G.
Henrot-Versille, S.
Hernandez-Monteagudo, C.
Herranz, D.
Hildebrandt, S. R.
Hivon, E.
Hobson, M.
Holmes, W. A.
Hornstrup, A.
Hovest, W.
Huang, Z.
Huffenberger, K. M.
Hurier, G.
Jaffe, A. H.
Jaffe, T. R.
Jones, W. C.
Juvela, M.
Keihanen, E.
Keskitalo, R.
Kisner, T. S.
Kneissl, R.
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Kurki-Suonio, H.
Lagache, G.
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Lasenby, A.
Lattanzi, M.
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Leonardi, R.
Lesgourgues, J.
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Liguori, M.
Lilje, P. B.
Linden-Vornle, M.
Lopez-Caniego, M.
Lubin, P. M.
Macias-Perez, J. F.
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Marchini, A.
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Reinecke, M.
Remazeilles, M.
Renault, C.
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Ristorcelli, I.
Rocha, G.
Rosset, C.
Rossetti, M.
Roudier, G.
d'Orfeui, B. Rouille
Rowan-Robinson, M.
Rubino-Martin, J. A.
Rusholme, B.
Said, N.
Salvatelli, V.
Salvati, L.
Sandri, M.
Santos, D.
Savelainen, M.
Savini, G.
Scott, D.
Seiffert, M. D.
Serra, P.
Shellard, E. P. S.
Spencer, L. D.
Spinelli, M.
Stolyarov, V.
Stompor, R.
Sudiwala, R.
Sunyaev, R.
Sutton, D.
Suur-Uski, A. -S.
Sygnet, J. -F.
Tauber, J. A.
Terenzi, L.
Toffolatti, L.
Tomasi, M.
Tristram, M.
Trombetti, T.
Tucci, M.
Tuovinen, J.
Turler, M.
Umana, G.
Valenziano, L.
Valiviita, J.
Van Tent, F.
Vielva, P.
Villa, F.
Wade, L. A.
Wandelt, B. D.
Wehus, I. K.
White, M.
White, S. D. M.
Wilkinson, A.
Yvon, D.
Zacchei, A.
Zonca, A.
CA Planck Collaboration
TI Planck 2015 results XIII. Cosmological parameters
SO ASTRONOMY & ASTROPHYSICS
LA English
DT Article
DE cosmology: observations; cosmology: theory; cosmic background radiation;
cosmological parameters
ID PROBE WMAP OBSERVATIONS; BARYON ACOUSTIC-OSCILLATIONS; MICROWAVE
BACKGROUND ANISOTROPIES; REDSHIFT-SPACE DISTORTIONS; SOUTH-POLE
TELESCOPE; ANNIHILATING DARK-MATTER; SPT-SZ SURVEY; CMB SPECTRAL
DISTORTIONS; ANGULAR POWER SPECTRUM; LARGE-SCALE STRUCTURE
AB This paper presents cosmological results based on full-mission Planck observations of temperature and polarization anisotropies of the cosmic microwave background (CMB) radiation. Our results are in very good agreement with the 2013 analysis of the Planck nominal-mission temperature data, but with increased precision. The temperature and polarization power spectra are consistent with the standard spatially-flat 6-parameter Lambda CDM cosmology with a power-law spectrum of adiabatic scalar perturbations (denoted "base Lambda CDM" in this paper). From the Planck temperature data combined with Planck lensing, for this cosmology we find a Hubble constant, H-0 = (67.8 +/- 0.9) km s(-1)Mpc(-1), a matter density parameter Omega(m) = 0.308 +/- 0.012, and a tilted scalar spectral index with ns = 0.968 +/- 0.006, consistent with the 2013 analysis. Note that in this abstract we quote 68% confidence limits on measured parameters and 95% upper limits on other parameters. We present the first results of polarization measurements with the Low Frequency Instrument at large angular scales. Combined with the Planck temperature and lensing data, these measurements give a reionization optical depth of tau = 0.066 +/- 0.016, corresponding to a reionization redshift of z(re) = 8.8(-1.4)(+1.7) These results are consistent with those from WMAP polarization measurements cleaned for dust emission using 353-GHz polarization maps from the High Frequency Instrument. We find no evidence for any departure from base Lambda CDM in the neutrino sector of the theory; for example, combining Planck observations with other astrophysical data we find N-eff = 3.15 +/- 0.23 for the effective number of relativistic degrees of freedom, consistent with the value N-eff = 3.046 of the Standard Model of particle physics. The sum of neutrino masses is constrained to Sigma m(v) < 0.23 eV. The spatial curvature of our Universe is found to be very close to zero, with vertical bar Omega(K)vertical bar < 0.005. Adding a tensor component as a single-parameter extension to base Lambda CDM we find an upper limit on the tensor-to-scalar ratio of r(0.002) < 0.11, consistent with the Planck 2013 results and consistent with the B-mode polarization constraints from a joint analysis of BICEP2, Keck Array, and Planck (BKP) data. Adding the BKP B-mode data to our analysis leads to a tighter constraint of r(0.002) < 0.09 and disfavours inflationary models with a V(phi) proportional to phi(2) potential. The addition of Planck polarization data leads to strong constraints on deviations from a purely adiabatic spectrum of fluctuations. We find no evidence for any contribution from isocurvature perturbations or from cosmic defects. Combining Planck data with other astrophysical data, including Type Ia supernovae, the equation of state of dark energy is constrained to w = -1.006 +/- 0.045, consistent with the expected value for a cosmological constant. The standard big bang nucleosynthesis predictions for the helium and deuterium abundances for the best-fit Planck base Lambda CDM cosmology are in excellent agreement with observations. We also constraints on annihilating dark matter and on possible deviations from the standard recombination history. In neither case do we find no evidence for new physics.
The Planck results for base Lambda CDM are in good agreement with baryon acoustic oscillation data and with the JLA sample of Type Ia supernovae. However, as in the 2013 analysis, the amplitude of the fluctuation spectrum is found to be higher than inferred from some analyses of rich cluster counts and weak gravitational lensing. We show that these tensions cannot easily be resolved with simple modifications of the base Lambda CDM cosmology. Apart from these tensions, the base Lambda CDM cosmology provides an excellent description of the Planck CMB observations and many other astrophysical data sets.
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[Naselsky, P.] Univ Copenhagen, Niels Bohr Inst, Blegdamsvej 17, DK-1165 Copenhagen, Denmark.
[Gerbino, M.; Gudmundsson, J. E.] Nordita Nord Inst Theoret Phys, Roslagstullsbacken 23, S-10691 Stockholm, Sweden.
[Savini, G.] UCL, Opt Sci Lab, Gower St, London, England.
[Farhang, M.] Shahid Beheshti Univ, Dept Phys, Tehran, Iran.
[Baccigalupi, C.; Bielewicz, P.; Danese, L.; de Zotti, G.; Paci, F.; Perrotta, F.] SISSA, Astrophys Sect, Via Bonomea 265, I-34136 Trieste, Italy.
[Terenzi, L.] Univ E Campus, SMARTEST Res Ctr, Via Isimbardi 10, Novedrate, CO, Italy.
[Ade, P. A. R.; Munshi, D.; Spencer, L. D.; Sudiwala, R.] Cardiff Univ, Sch Phys & Astron, Queens Bldg, Cardiff CF24 3AA, S Glam, Wales.
[Moss, A.] Univ Nottingham, Sch Phys & Astron, Nottingham NG7 2RD, England.
[Bouchet, F. R.; Di Valentino, E.] Sorbonne Univ UPMC, UMR7095, Inst Astrophys Paris, 98bis Blvd Arago, F-75014 Paris, France.
[Sunyaev, R.] Russian Acad Sci, Space Res Inst IKI, Profsoyuznaya Str 84-32, Moscow 117997, Russia.
[Borrill, J.] Univ Calif Berkeley, Space Sci Lab, Berkeley, CA 94720 USA.
[Stolyarov, V.] Russian Acad Sci, Special Astrophys Observ, Karachai Cherkessian Rep 369167, Zelenchukskiy R, Russia.
[Church, S.] Stanford Univ, Dept Phys, Varian Phys Bldg,382 via Pueblo Mall, Stanford, CA 94305 USA.
[Calabrese, E.; Dunkley, J.] Univ Oxford, Subdept Astrophys, Keble Rd, Oxford OX1 3RH, England.
[Hamann, J.] Univ Sydney, Sch Phys A28, Sydney Inst Astron, Sydney, NSW 2006, Australia.
[Gerbino, M.; Gudmundsson, J. E.] Stockholm Univ, AlbaNova, Dept Phys, Oskar Klein Ctr Cosmoparticle Phys, S-10691 Stockholm, Sweden.
[Hamann, J.; Lesgourgues, J.] CERN, PH TH, Div Theory, CH-1211 Geneva 23, Switzerland.
[Benabed, K.; Benoit-Levy, A.; Colombi, S.; Elsner, F.; Hivon, E.; Prunet, S.; Wandelt, B. D.] UPMC Univ Paris 06, UMR 7095, 98bis Blvd Arago, F-75014 Paris, France.
[Banday, A. J.; Bernard, J. -P.; Forni, O.; Giard, M.; Jaffe, T. R.; Montier, L.; Pointecouteau, E.; Ristorcelli, I.] Univ Toulouse, UPS OMP, IRAP, F-31028 Toulouse 4, France.
[Reach, W. T.] Univ Space Res Assoc, Stratospher Observ Infrared Astron, MS 232-11, Moffett Field, CA 94035 USA.
[Dolag, K.] Ludwig Maximilian Univ Munich, Univ Observ, Scheinerstr1, D-81679 Munich, Germany.
[Battaner, E.] Univ Granada, Dept Fis Teor & Cosmos, Fac Ciencias, Granada 11071, Spain.
[Battaner, E.] Univ Granada, Inst Carlos Fis Teer & Computac 1, Granada 11071, Spain.
[Martinelli, M.] Heidelberg Univ, Inst Theoret Phys, Philosophenweg 16, D-69120 Heidelberg, Germany.
[Gorski, K. M.] Univ Warsaw Observ, Aleje Ujazdowskie 4, PL-00478 Warsaw, Poland.
RP Efstathiou, G (reprint author), Univ Cambridge, Inst Astron, Madingley Rd, Cambridge CB3 0HA, England.; Efstathiou, G (reprint author), Kavli Inst Cosmol Cambridge, Madingley Rd, Cambridge CB3 0HA, England.
EM gpe@ast.cam.ac.uk
RI Lahteenmaki, Anne/L-5987-2013; Gerbino, Martina/E-4029-2017; Barreiro,
Rita Belen/N-5442-2014; bonavera, laura/E-9368-2017; Gonzalez-Nuevo,
Joaquin/I-3562-2014; Herranz, Diego/K-9143-2014; Colombo,
Loris/J-2415-2016;
OI Pierpaoli, Elena/0000-0002-7957-8993; Juvela, Mika/0000-0002-5809-4834;
Huang, Zhiqi/0000-0002-1506-1063; TERENZI, LUCA/0000-0001-9915-6379;
Reach, William/0000-0001-8362-4094; Valiviita,
Jussi/0000-0001-6225-3693; Toffolatti, Luigi/0000-0003-2645-7386; Lilje,
Per/0000-0003-4324-7794; Paoletti, Daniela/0000-0003-4761-6147; Nati,
Federico/0000-0002-8307-5088; Savini, Giorgio/0000-0003-4449-9416;
Martinelli, Matteo/0000-0002-6943-7732; Stolyarov,
Vladislav/0000-0001-8151-828X; Gerbino, Martina/0000-0002-3538-1283;
Barreiro, Rita Belen/0000-0002-6139-4272; bonavera,
laura/0000-0001-8039-3876; Gonzalez-Nuevo, Joaquin/0000-0003-1354-6822;
Herranz, Diego/0000-0003-4540-1417; Colombo, Loris/0000-0003-4572-7732;
Hivon, Eric/0000-0003-1880-2733; Kurki-Suonio,
Hannu/0000-0002-4618-3063; Zacchei, Andrea/0000-0003-0396-1192
FU ESA; CNES (France); CNRS/INSU-IN2P3-INP (France); ASI (Italy); CNR
(Italy); INAF (Italy); NASA (USA); DoE (USA); STFC (UK); UKSA (UK); CSIC
(Spain); MINECO (Spain); JA (Spain); RES (Spain); Tekes (Finland); AoF
(Finland); CSC (Finland); DLR (Germany); MPG (Germany); CSA (Canada);
DTU Space (Denmark); SER/SSO (Switzerland); RCN (Norway); SFI (Ireland);
FCT/MCTES (Portugal); ERC (EU); PRACE (EU); European Research Council
under the European Union's Seventh Framework Programme (FP)/ERC Grant
[616170]; UK Science and Technology Facilities Council [ST/L000652/1];
UK BIS National E-infrastructure capital grants
FX The Planck Collaboration acknowledges the support of: ESA; CNES and
CNRS/INSU-IN2P3-INP (France); ASI, CNR, and INAF (Italy); NASA and DoE
(USA); STFC and UKSA (UK); CSIC, MINECO, JA, and RES (Spain); Tekes,
AoF, and CSC (Finland); DLR and MPG (Germany); CSA (Canada); DTU Space
(Denmark); SER/SSO (Switzerland); RCN (Norway); SFI (Ireland); FCT/MCTES
(Portugal); ERC and PRACE (EU). A description of the Planck
Collaboration and a list of its members, indicating which technical or
scientific activities they have been involved in, can be found at
http://www.cosmos.esa.int/web/planck/planck-collaboration. Some of the
results in this paper have been derived using the HEALPix package. The
research leading to these results has received funding from the European
Research Council under the European Union's Seventh Framework Programme
(FP/2007-2013)/ERC Grant Agreement No. [616170] and from the UK Science
and Technology Facilities Council [grant number ST/L000652/1]. Part of
this work was undertaken on the STFC DiRAC HPC Facilities at the
University of Cambridge, funded by UK BIS National E-infrastructure
capital grants, and on the Andromeda cluster of the University of
Geneva. A large set of cosmological parameter constraints from different
data combinations, and including many separate extensions to the
6-parameter base Lambda CDM model, are available at
http://pla.esac.esa.int/pla/#cosmology.
NR 369
TC 237
Z9 237
U1 6
U2 6
PU EDP SCIENCES S A
PI LES ULIS CEDEX A
PA 17, AVE DU HOGGAR, PA COURTABOEUF, BP 112, F-91944 LES ULIS CEDEX A,
FRANCE
SN 1432-0746
J9 ASTRON ASTROPHYS
JI Astron. Astrophys.
PD OCT
PY 2016
VL 594
AR A13
DI 10.1051/0004-6361/201525830
PG 63
WC Astronomy & Astrophysics
SC Astronomy & Astrophysics
GA DZ4MG
UT WOS:000385832200013
ER
PT J
AU Aghanim, N
Arnaud, M
Ashdown, M
Aumont, J
Baccigalupi, C
Banday, AJ
Barreiro, RB
Bartlett, JG
Bartolo, N
Battaner, E
Battye, R
Benabed, K
Benoit, A
Benoit-Levy, A
Bernard, JP
Bersanelli, M
Bielewicz, P
Bock, JJ
Bonaldi, A
Bonavera, L
Bond, JR
Borrill, J
Bouchet, FR
Burigana, C
Butler, RC
Calabrese, E
Cardoso, JF
Catalano, A
Challinor, A
Chiang, HC
Christensen, PR
Churazov, E
Clements, DL
Colombo, LPL
Combet, C
Comis, B
Coulais, A
Crill, BP
Curto, A
Cuttaia, F
Danese, L
Davies, RD
Davis, RJ
de Bernardis, P
de Rosa, A
de Zotti, G
Delabrouille, J
Desert, FX
Dickinson, C
Diego, JM
Dolag, K
Dole, H
Donzelli, S
Dore, O
Douspis, M
Ducout, A
Dupac, X
Efstathiou, G
Elsner, F
Ensslin, TA
Eriksen, HK
Fergusson, J
Finelli, F
Forni, O
Frailis, M
Fraisse, AA
Franceschi, E
Frejse, A
Galeotta, S
Galli, S
Ganga, K
Genova-Santos, RT
Giard, M
Gonzalez-Nuevo, J
Gorski, KM
Gregorio, A
Gruppuso, A
Gudmundsson, JE
Hansen, FK
Harrison, DL
Henrot-Versille, S
Hernandez-Monteagudo, C
Herranz, D
Hildebrandt, SR
Hivon, E
Holmes, WA
Hornstrup, A
Huffenberger, KM
Hurier, G
Jaffe, AH
Jones, WC
Juvela, M
Keihanen, E
Keskitalo, R
Kneissl, R
Knoche, J
Kunz, M
Kurki-Suonio, H
Lacasa, F
Lagache, G
Lahteenmaki, A
Lamarre, JM
Lasenby, A
Lattanzi, M
Leonardi, R
Lesgourgues, J
Levrier, F
Liguori, M
Lilje, PB
Linden-Vornle, M
Lopez-Caniego, M
Macias-Perez, JF
Maffei, B
Maggie, G
Maino, D
Mandolesi, N
Mangilli, A
Maris, M
Martin, PG
Martinez-Gonzalez, E
Masi, S
Matarrese, S
Melchiorri, A
Melin, JB
Migliaccio, M
Miville-Deschenes, MA
Moneti, A
Montier, L
Morgante, G
Mortlock, D
Munshi, D
Murphy, JA
Naselsky, P
Nati, F
Natoli, P
Noviello, F
Novikov, D
Novikov, I
Paci, F
Pagano, L
Pajot, F
Paoletti, D
Pasian, F
Patanchon, G
Perdereau, O
Perotto, L
Pettorino, V
Piacentini, F
Piat, M
Pierpaoli, E
Pietrobon, D
Plaszczynski, S
Pointecouteau, E
Polenta, G
Ponthieu, N
Pratt, GW
Prunet, S
Puget, JL
Rachen, JP
Reinecke, M
Remazeilles, M
Renault, C
Renzi, A
Ristorcelli, I
Rocha, G
Rossetti, M
Roudier, G
Rubino-Martin, JA
Rusholme, B
Sandri, M
Santos, D
Sauve, A
Savelainen, M
Savini, G
Scott, D
Spencer, LD
Stolyarov, V
Stompor, R
Sunyaev, R
Sutton, D
Suur-Uski, AS
Sygnet, JF
Tauber, JA
Terenzi, L
Toffolatti, L
Tomasi, M
Tramonte, D
Tristram, M
Tucci, M
Tuovinen, J
Valenziano, L
Valiviita, J
Van Tent, B
Vielva, P
Villa, F
Wade, LA
Wandelt, BD
Wehus, IK
Yvon, D
Zacchei, A
Zonca, A
AF Aghanim, N.
Arnaud, M.
Ashdown, M.
Aumont, J.
Baccigalupi, C.
Banday, A. J.
Barreiro, R. B.
Bartlett, J. G.
Bartolo, N.
Battaner, E.
Battye, R.
Benabed, K.
Benoit, A.
Benoit-Levy, A.
Bernard, J. -P.
Bersanelli, M.
Bielewicz, P.
Bock, J. J.
Bonaldi, A.
Bonavera, L.
Bond, J. R.
Borrill, J.
Bouchet, F. R.
Burigana, C.
Butler, R. C.
Calabrese, E.
Cardoso, J. -F.
Catalano, A.
Challinor, A.
Chiang, H. C.
Christensen, P. R.
Churazov, E.
Clements, D. L.
Colombo, L. P. L.
Combet, C.
Comis, B.
Coulais, A.
Crill, B. P.
Curto, A.
Cuttaia, F.
Danese, L.
Davies, R. D.
Davis, R. J.
de Bernardis, P.
de Rosa, A.
de Zotti, G.
Delabrouille, J.
Desert, F. -X.
Dickinson, C.
Diego, J. M.
Dolag, K.
Dole, H.
Donzelli, S.
Dore, O.
Douspis, M.
Ducout, A.
Dupac, X.
Efstathiou, G.
Elsner, F.
Ensslin, T. A.
Eriksen, H. K.
Fergusson, J.
Finelli, F.
Forni, O.
Frailis, M.
Fraisse, A. A.
Franceschi, E.
Frejse, A.
Galeotta, S.
Galli, S.
Ganga, K.
Genova-Santos, R. T.
Giard, M.
Gonzalez-Nuevo, J.
Gorski, K. M.
Gregorio, A.
Gruppuso, A.
Gudmundsson, J. E.
Hansen, F. K.
Harrison, D. L.
Henrot-Versille, S.
Hernandez-Monteagudo, C.
Herranz, D.
Hildebrandt, S. R.
Hivon, E.
Holmes, W. A.
Hornstrup, A.
Huffenberger, K. M.
Hurier, G.
Jaffe, A. H.
Jones, W. C.
Juvela, M.
Keihanen, E.
Keskitalo, R.
Kneissl, R.
Knoche, J.
Kunz, M.
Kurki-Suonio, H.
Lacasa, F.
Lagache, G.
Lahteenmaki, A.
Lamarre, J. -M.
Lasenby, A.
Lattanzi, M.
Leonardi, R.
Lesgourgues, J.
Levrier, F.
Liguori, M.
Lilje, P. B.
Linden-Vornle, M.
Lopez-Caniego, M.
Macias-Perez, J. F.
Maffei, B.
Maggie, G.
Maino, D.
Mandolesi, N.
Mangilli, A.
Maris, M.
Martin, P. G.
Martinez-Gonzalez, E.
Masi, S.
Matarrese, S.
Melchiorri, A.
Melin, J. -B.
Migliaccio, M.
Miville-Deschenes, M. -A.
Moneti, A.
Montier, L.
Morgante, G.
Mortlock, D.
Munshi, D.
Murphy, J. A.
Naselsky, P.
Nati, F.
Natoli, P.
Noviello, F.
Novikov, D.
Novikov, I.
Paci, F.
Pagano, L.
Pajot, F.
Paoletti, D.
Pasian, F.
Patanchon, G.
Perdereau, O.
Perotto, L.
Pettorino, V.
Piacentini, F.
Piat, M.
Pierpaoli, E.
Pietrobon, D.
Plaszczynski, S.
Pointecouteau, E.
Polenta, G.
Ponthieu, N.
Pratt, G. W.
Prunet, S.
Puget, J. -L.
Rachen, J. P.
Reinecke, M.
Remazeilles, M.
Renault, C.
Renzi, A.
Ristorcelli, I.
Rocha, G.
Rossetti, M.
Roudier, G.
Rubino-Martin, J. A.
Rusholme, B.
Sandri, M.
Santos, D.
Sauve, A.
Savelainen, M.
Savini, G.
Scott, D.
Spencer, L. D.
Stolyarov, V.
Stompor, R.
Sunyaev, R.
Sutton, D.
Suur-Uski, A. -S.
Sygnet, J. -F.
Tauber, J. A.
Terenzi, L.
Toffolatti, L.
Tomasi, M.
Tramonte, D.
Tristram, M.
Tucci, M.
Tuovinen, J.
Valenziano, L.
Valiviita, J.
Van Tent, B.
Vielva, P.
Villa, F.
Wade, L. A.
Wandelt, B. D.
Wehus, I. K.
Yvon, D.
Zacchei, A.
Zonca, A.
CA Planck Collaboration
TI Planck 2015 results XXII. A map of the thermal Sunyaev-Zeldovich effect
SO ASTRONOMY & ASTROPHYSICS
LA English
DT Article
DE large-scale structure of Universe; cosmology: observations
ID ANGULAR POWER SPECTRUM; SPT-SZ SURVEY; MICROWAVE BACKGROUND MAPS; POLE
TELESCOPE SURVEY; GALAXY CLUSTERS; X-RAY; COSMOLOGICAL PARAMETERS; POINT
SOURCES; DATA SETS; CMB
AB We have constructed all-sky Compton parameters maps, y-maps, of the thermal Sunyaev-Zeldovich (tSZ) effect by applying specifically tailored component separation algorithms to the 30 to 857 GHz frequency channel maps from the Planck satellite. These reconstructed y-maps are delivered as part of the Planck 2015 release. The y-maps are characterized in terms of noise properties and residual foreground contamination, mainly thermal dust emission at large angular scales, and cosmic infrared background and extragalactic point sources at small angular scales. Specific masks are defined to minimize foreground residuals and systematics. Using these masks, we compute the y-map angular power spectrum and higher order statistics. From these we conclude that the y-map is dominated by tSZ signal in the multipole range, 20 < l < 600. We compare the measured tSZ power spectrum and higher order statistics to various physically motivated models and discuss the implications of our results in terms of cluster physics and cosmology.
C1 [Bartlett, J. G.; Cardoso, J. -F.; Delabrouille, J.; Ganga, K.; Patanchon, G.; Piat, M.; Remazeilles, M.; Roudier, G.; Stompor, R.] Univ Paris Diderot, APC, CNRS IN2P3, CEA Lrfu,Observ Paris,Sorbonne Paris Cite, 10 Rue Alice Domon & Leonie Duquet, F-75205 Paris 13, France.
[Lahteenmaki, A.] Aalto Univ, Metsahovi Radio Observ, POB 13000, Aalto 00076, Finland.
[Lahteenmaki, A.] Aalto Univ, Dept Radio Sci & Engn, POB 13000, Aalto 00076, Finland.
[Kunz, M.] African Inst Math Sci, 6-8 Melrose Rd, ZA-7945 Cape Town, South Africa.
[Natoli, P.; Polenta, G.] Agenzia Spaziale Italiana, Sci Data Ctr, Via Politecn Snc, I-00133 Rome, Italy.
[Lagache, G.] Aix Marseille Univ, CNRS, LAM, UMR 7326, F-13388 Marseille, France.
[Ashdown, M.; Curto, A.; Lasenby, A.; Stolyarov, V.] Univ Cambridge, Cavendish Lab, Astrophys Grp, Cambridge CB3 0HE, England.
[Chiang, H. C.] Univ KwaZulu Natal, Sch Math Stat & Comp Sci, Astrophys & Cosmol Res Unit, Westville Campus,Private Bag X54001, ZA-4000 Durban, South Africa.
[Kneissl, R.] ALMA Santiago Cent Off, Atacama Large Millimeter Submillimeter Array, Alonso Cordova 3107,763 0355 Casilla, Santiago, Chile.
[Martin, P. G.; Miville-Deschenes, M. -A.] Univ Toronto, CITA, 60 St George St, Toronto, ON M5S 2S1, Canada.
[Banday, A. J.; Bernard, J. -P.; Bielewicz, P.; Forni, O.; Giard, M.; Montier, L.; Pointecouteau, E.; Ristorcelli, I.; Sauve, A.] IRAP, CNRS, 9 Ave colonel Roche,BP 44346, F-31028 Toulouse 4, France.
[Tuovinen, J.] Trinity Coll Dublin, CRANN, Dublin 2, Ireland.
[Bock, J. J.; Crill, B. P.; Dore, O.; Hildebrandt, S. R.; Rocha, G.] CALTECH, Pasadena, CA 91125 USA.
[Challinor, A.; Fergusson, J.] Univ Cambridge, DAMTP, Ctr Theoret Cosmol, Wilberforce Rd, Cambridge CB3 0WA, England.
[Hernandez-Monteagudo, C.] CEFCA, Plaza San Juan,1,Planta 2, Teruel 44001, Spain.
[Borrill, J.; Keskitalo, R.] Lawrence Berkeley Natl Lab, Computat Cosmol Ctr, Berkeley, CA 94720 USA.
[Melin, J. -B.; Yvon, D.] CEA Saclay, DSM, Irfu, SPP, Gif Sur Yvette, France.
[Hornstrup, A.; Linden-Vornle, M.] Tech Univ Denmark, Natl Space Inst, DTU Space, Elektrovej 327, DK-2800 Lyngby, Denmark.
[Kunz, M.; Tucci, M.] Univ Geneva, Dept Phys Theor, 24 Quai E Ansermet, CH-1211 Geneva 4, Switzerland.
[Toffolatti, L.] Univ Oviedo, Dept Fis, Avda Calvo Sotelo S-N, Oviedo 33003, Spain.
[Rachen, J. P.] Radboud Univ Nijmegen, IMAPP, Dept Astrophys, POB 9010, NL-6500 GL Nijmegen, Netherlands.
[Scott, D.] Univ British Columbia, Dept Phys & Astron, 6224 Agr Rd, Vancouver, BC, Canada.
[Pierpaoli, E.] Univ Southern Calif, Dana & David Dornsife Coll Letter Arts & Sci, Dept Phys & Astron, Los Angeles, CA 90089 USA.
[Benoit-Levy, A.; Elsner, F.] UCL, Dept Phys & Astron, London WC1E 6BT, England.
[Huffenberger, K. M.; Savelainen, M.; Suur-Uski, A. -S.] Florida State Univ, Dept Phys, Keen Phys Bldg,77 Chieftan Way, Tallahassee, FL 32306 USA.
[Juvela, M.; Keihanen, E.; Kurki-Suonio, H.; Valiviita, J.] Univ Helsinki, Dept Phys, Gustaf Hallstromin Katu 2a, 00014 Helsinki, Finland.
[Chiang, H. C.; Colombo, L. P. L.; Fraisse, A. A.; Gudmundsson, J. E.; Jones, W. C.; Nati, F.] Princeton Univ, Dept Phys, Princeton, NJ 08544 USA.
[Zonca, A.] Univ Calif Santa Barbara, Dept Phys, Santa Barbara, CA 93106 USA.
[Wandelt, B. D.] Univ Illinois, Dept Phys, 1110 West Green St, Urbana, IL 61801 USA.
[Bartolo, N.; Liguori, M.; Matarrese, S.] Univ Padua, Dipartimento Fis & Astron G Galilei, Via Marzolo 8, I-35131 Padua, Italy.
[Burigana, C.; Lattanzi, M.; Mandolesi, N.; Natoli, P.] Univ Ferrara, Dipartimento Fis & Sci Terra, Via Saragat 1, I-44122 Ferrara, Italy.
[de Bernardis, P.; Masi, S.; Melchiorri, A.; Pagano, L.; Piacentini, F.] Univ Roma La Sapienza, Dipartimento Fis, Ple A Moro 2, I-00185 Rome, Italy.
[Bersanelli, M.; Maino, D.; Rossetti, M.; Tomasi, M.] Univ Milan, Dipartimento Fis, Via Celoria 16, I-20133 Milan, Italy.
[Gregorio, A.] Univ Trieste, Dipartimento Fis, Via A Valerio 2, I-34127 Trieste, Italy.
[Renzi, A.] Univ Roma Tor Vergata, Dipartimento Matemat, Via Ric Sci 1, I-00133 Rome, Italy.
[Christensen, P. R.; Naselsky, P.] Niels Bohr Inst, Discovery Ctr, Blegdamsvej 17, DK-2100 Copenhagen, Denmark.
[Genova-Santos, R. T.; Rubino-Martin, J. A.; Tramonte, D.] Univ La Laguna, Dept Astrofis, E-38206 Tenerife, Spain.
[Kneissl, R.] ESO Vitacura, European So Observ, Alonso Cordova 3107,Casilla 19001, Santiago, Chile.
[Dupac, X.; Leonardi, R.; Lopez-Caniego, M.] European Space Agcy, ESAC, Planck Sci Off, Camino Bajo Castillo,S-N, Madrid 28692, Spain.
[Tauber, J. A.] European Space Agcy, Estec, Keplerlaan 1, NL-2201 AZ Noordwijk, Netherlands.
[Terenzi, L.] Univ E Campus, Fac Ingn, Via Isimbardi 10, I-22060 Novedrate, CO, Italy.
[Matarrese, S.] Ist Nazl Fis Nucl, Gran Sasso Sci Inst, Viale F Crispi 7, I-67100 Laquila, Italy.
[Pettorino, V.] HGSFP, Philosophenweg 16, D-69120 Heidelberg, Germany.
[Pettorino, V.] Heidelberg Univ, Dept Theoret Phys, Philosophenweg 16, D-69120 Heidelberg, Germany.
[Kurki-Suonio, H.; Lahteenmaki, A.; Savelainen, M.; Suur-Uski, A. -S.; Valiviita, J.] Univ Helsinki, Helsinki Inst Phys, Gustaf Hallstromin Katu 2, FIN-00014 Helsinki, Finland.
[Lacasa, F.] Univ Estadual Paulista, Inst Fis Teor, ICTP South Amer Inst Fundamental Res, BR-01140070 Sao Paulo, Brazil.
[de Zotti, G.] INAF Osservatorio Astron Padova, Vicolo Osservatorio 5, I-35122 Padua, Italy.
[Polenta, G.] INAF Osservatorio Astron Roma, Via Frascati 33, I-00040 Monte Porzio Catone, Italy.
[Frailis, M.; Galeotta, S.; Gregorio, A.; Maggie, G.; Maris, M.; Pasian, F.; Zacchei, A.] INAF Osservatorio Astron Trieste, Via GB Tiepolo 11, I-40127 Trieste, Italy.
[Burigana, C.; Butler, R. C.; Cuttaia, F.; de Rosa, A.; Finelli, F.; Franceschi, E.; Gruppuso, A.; Mandolesi, N.; Morgante, G.; Natoli, P.; Paoletti, D.; Perdereau, O.; Sandri, M.; Terenzi, L.; Toffolatti, L.; Valenziano, L.; Villa, F.] INAF IASF Bologna, Via Gobetti 101, I-40129 Bologna, Italy.
[Bersanelli, M.; Donzelli, S.; Maino, D.; Rossetti, M.; Tomasi, M.] INAF IASF Milano, Via E Bassini 15, I-20133 Milan, Italy.
[Burigana, C.; Finelli, F.; Paoletti, D.] Ist Nazl Fis Nucl, Sez Bologna, Via Irnerio 46, I-40126 Bologna, Italy.
[Melchiorri, A.; Pagano, L.] Univ Roma Sapienza, Sez Roma 1, INFN, Ple Aldo Moro 2, I-00185 Rome, Italy.
[Renzi, A.] Univ Roma Tor Vergata, Sez Roma 2, INFN, Via Ric Sci 1, I-00185 Rome, Italy.
[Gregorio, A.] Ist Nazl Fis Nucl, Via Valerio 2, I-34127 Trieste, Italy.
[Desert, F. -X.; Ponthieu, N.] Univ Grenoble Alpes, IPAG, CNRS, F-38000 Grenoble, France.
[Clements, D. L.; Ducout, A.; Jaffe, A. H.; Mortlock, D.] Imperial Coll London, Astrophys Grp, Blackett Lab, Prince Consort Rd, London SW7 2AZ, England.
[Rusholme, B.] CALTECH, Infrared Proc & Anal Ctr, Pasadena, CA 91125 USA.
[Benoit, A.] Univ Joseph Fourier Grenoble I, CNRS, Inst Neel, 25 Rue Martyrs, Grenoble, France.
[Dole, H.] Inst Univ France, 103 Bd St Michel, F-75005 Paris, France.
[Aghanim, N.; Aumont, J.; Dole, H.; Douspis, M.; Hurier, G.; Kunz, M.; Lacasa, F.; Lagache, G.; Mangilli, A.; Miville-Deschenes, M. -A.; Pajot, F.; Ponthieu, N.; Puget, J. -L.; Remazeilles, M.] Univ Paris Sud 11, UMR 8617, CNRS, Inst Astrophys Spatiale, Batiment 121, F-91405 Orsay, France.
[Benabed, K.; Benoit-Levy, A.; Bouchet, F. R.; Cardoso, J. -F.; Ducout, A.; Elsner, F.; Galli, S.; Hivon, E.; Moneti, A.; Prunet, S.; Sygnet, J. -F.; Wandelt, B. D.] Inst Astrophys Paris, CNRS, UMR 7095, 98bis Blvd Arago, F-75014 Paris, France.
[Challinor, A.; Efstathiou, G.; Harrison, D. L.; Migliaccio, M.; Sutton, D.] Univ Cambridge, Inst Astron, Madingley Rd, Cambridge CB3 0HA, England.
[Eriksen, H. K.; Hansen, F. K.; Lilje, P. B.] Univ Oslo, Inst Theoret Astrophys, N-0371 Oslo, Norway.
[Genova-Santos, R. T.; Rubino-Martin, J. A.; Tramonte, D.] Inst Astrofis Canarias, C Via Lactea S-N, Tenerife 38205, Spain.
[Barreiro, R. B.; Bonavera, L.; Curto, A.; Diego, J. M.; Gonzalez-Nuevo, J.; Herranz, D.; Lopez-Caniego, M.; Martinez-Gonzalez, E.; Toffolatti, L.; Vielva, P.] CSIC Univ Cantabria, Inst Fis Cantabria, Avda Castros S-N, Santander 39005, Spain.
[Bartolo, N.; Liguori, M.; Matarrese, S.] Ist Nazl Fis Nucl, Sez Padova, Via Marzolo 8, I-35131 Padua, Italy.
[Bartlett, J. G.; Bock, J. J.; Colombo, L. P. L.; Crill, B. P.; Dore, O.; Hildebrandt, S. R.; Holmes, W. A.; Pietrobon, D.; Rocha, G.; Roudier, G.; Wade, L. A.; Wehus, I. K.] CALTECH, Jet Prop Lab, 4800 Oak Grove Dr, Pasadena, CA USA.
[Battye, R.; Bonaldi, A.; Davies, R. D.; Davis, R. J.; Dickinson, C.; Maffei, B.; Noviello, F.; Remazeilles, M.] Univ Manchester, Sch Phys & Astron, Jodrell Bank Ctr Astrophys, Alan Turing Bldg,Oxford Rd, Manchester M13 9PL, Lancs, England.
[Ashdown, M.; Challinor, A.; Harrison, D. L.; Lasenby, A.; Migliaccio, M.; Stolyarov, V.; Sutton, D.] Kavli Inst Cosmol Cambridge, Madingley Rd, Cambridge CB3 0HA, England.
[Gorski, K. M.; Henrot-Versille, S.; Mangilli, A.; Perdereau, O.; Plaszczynski, S.; Tristram, M.] Univ Paris 11, LAL, CNRS IN2P3, F-91898 Orsay, France.
[Lesgourgues, J.] Univ Savoie, LAPTh, CNRS, BP 110, F-74941 Annecy Le Vieux, France.
[Catalano, A.; Coulais, A.; Lamarre, J. -M.; Levrier, F.; Roudier, G.] Observ Paris, CNRS, LERMA, 61 Ave Observ, F-75014 Paris, France.
[Catalano, A.; Coulais, A.; Lamarre, J. -M.; Levrier, F.; Roudier, G.] Univ Paris Diderot, CEA DSM, CNRS, Lab AIM,IRFU,Serv Astrophys,CEA Saclay, Bat 709, F-91191 Gif Sur Yvette, France.
[Cardoso, J. -F.] CNRS, UMR 5141, Lab Traitement & Commun Informat, 46 Rue Barrault, F-75634 Paris 13, France.
[Cardoso, J. -F.] Telecom ParisTech, 46 Rue Barrault, F-75634 Paris 13, France.
[Catalano, A.; Comis, B.; Macias-Perez, J. F.; Perotto, L.; Renault, C.; Santos, D.] Univ Grenoble Alpes, Lab Phys Subat & Cosmol, CNRS IN2P3, 53 Rue Martyrs, F-38026 Grenoble, France.
[Combet, C.; Van Tent, B.] Univ Paris Sud 11, Lab Phys Theor, Batiment 210, F-91405 Orsay, France.
[Combet, C.; Van Tent, B.] CNRS, Batiment 210, F-91405 Orsay, France.
[Novikov, D.; Novikov, I.] Russian Acad Sci, Lebedev Phys Inst, Astro Space Ctr, 84-32 Profsoyuznaya St,GSP 7, Moscow 117997, Russia.
[Churazov, E.; Dolag, K.; Ensslin, T. A.; Hernandez-Monteagudo, C.; Knoche, J.; Rachen, J. P.; Reinecke, M.; Sunyaev, R.] Max Planck Inst Astrophys, Karl Schwarzschild Str 1, D-85741 Garching, Germany.
[Murphy, J. A.] Natl Univ Ireland, Dept Expt Phys, Maynooth, Kildare, Ireland.
[Christensen, P. R.; Frejse, A.; Naselsky, P.; Novikov, I.] Niels Bohr Inst, Blegdamsvej 17, DK-2100 Copenhagen, Denmark.
[Savini, G.] UCL, Opt Sci Lab, Gower St, London WC1E 6BT, England.
[de Zotti, G.; Lesgourgues, J.] Ecole Polytech Fed Lausanne, SB ITP LPPC, CH-1015 Lausanne, Switzerland.
[Baccigalupi, C.; Bielewicz, P.; Danese, L.; Gonzalez-Nuevo, J.; Paci, F.] SISSA, Astrophys Sector, Via Bonomea 265, I-34136 Trieste, Italy.
[Munshi, D.; Spencer, L. D.] Cardiff Univ, Sch Phys & Astron, Queens Bldg, Cardiff CF24 3AA, S Glam, Wales.
[Bouchet, F. R.] UPMC, Sorbonne Univ, UMR7095, Inst Astrophys Paris, 98bis Blvd Arago, F-75014 Paris, France.
[Churazov, E.; Sunyaev, R.] Russian Acad Sci, Space Res Inst IKI, Profsoyuznaya Str,84-32, Moscow 117997, Russia.
[Borrill, J.] Univ Calif Berkeley, Space Sci Lab, Berkeley, CA 94720 USA.
[Stolyarov, V.] Russian Acad Sci, Special Astrophys Observ, Karachai Cherkessian Rep 369167, Zelenchukskiy R, Russia.
[Calabrese, E.] Univ Oxford, Subdept Astrophys, Keble Rd, Oxford OX1 3RH, England.
[Lesgourgues, J.] CERN, PH TH, Div Theory, CH-23 Geneva, Switzerland.
[Benabed, K.; Benoit-Levy, A.; Elsner, F.; Hivon, E.; Prunet, S.; Wandelt, B. D.] UPMC Univ Paris 06, UMR 7095, 98bis Blvd Arago, F-75014 Paris, France.
[Banday, A. J.; Bernard, J. -P.; Bielewicz, P.; Forni, O.; Giard, M.; Montier, L.; Pointecouteau, E.; Ristorcelli, I.; Sauve, A.] Univ Toulouse, UPS OMP, IRAP, F-31028 Toulouse 4, France.
[Dolag, K.] Ludwig Maximilian Univ Munich, Univ Observ, Scheinerstr 1, D-81679 Munich, Germany.
[Battaner, E.] Univ Granada, Dept Fis Teor & Cosmos, Fac Ciencias, Granada 18071, Spain.
[Battaner, E.] Univ Granada, Inst Carlos Fis Teor & Computac, Granada 18071, Spain.
[Gorski, K. M.] Univ Warsaw Observ, Aleje Ujazdowskie 4, PL-00478 Warsaw, Poland.
RP Remazeilles, M (reprint author), Univ Paris Diderot, APC, CNRS IN2P3, CEA Lrfu,Observ Paris,Sorbonne Paris Cite, 10 Rue Alice Domon & Leonie Duquet, F-75205 Paris 13, France.; Remazeilles, M (reprint author), Univ Paris Sud 11, UMR 8617, CNRS, Inst Astrophys Spatiale, Batiment 121, F-91405 Orsay, France.; Remazeilles, M (reprint author), Univ Manchester, Sch Phys & Astron, Jodrell Bank Ctr Astrophys, Alan Turing Bldg,Oxford Rd, Manchester M13 9PL, Lancs, England.; Comis, B (reprint author), Univ Grenoble Alpes, Lab Phys Subat & Cosmol, CNRS IN2P3, 53 Rue Martyrs, F-38026 Grenoble, France.
EM comis@lpscin2p3.fr; mathieu.remazeilles@manchester.ac.uk
RI Churazov, Eugene/A-7783-2013; Barreiro, Rita Belen/N-5442-2014;
bonavera, laura/E-9368-2017; Gonzalez-Nuevo, Joaquin/I-3562-2014;
Herranz, Diego/K-9143-2014; Colombo, Loris/J-2415-2016; Lahteenmaki,
Anne/L-5987-2013;
OI Barreiro, Rita Belen/0000-0002-6139-4272; bonavera,
laura/0000-0001-8039-3876; Gonzalez-Nuevo, Joaquin/0000-0003-1354-6822;
Herranz, Diego/0000-0003-4540-1417; Colombo, Loris/0000-0003-4572-7732;
TERENZI, LUCA/0000-0001-9915-6379; Stolyarov,
Vladislav/0000-0001-8151-828X; Valiviita, Jussi/0000-0001-6225-3693;
Kurki-Suonio, Hannu/0000-0002-4618-3063; Zacchei,
Andrea/0000-0003-0396-1192; Toffolatti, Luigi/0000-0003-2645-7386;
Lilje, Per/0000-0003-4324-7794; Paoletti, Daniela/0000-0003-4761-6147;
Nati, Federico/0000-0002-8307-5088; Savini, Giorgio/0000-0003-4449-9416;
Pierpaoli, Elena/0000-0002-7957-8993; Juvela, Mika/0000-0002-5809-4834
FU CNES (France); CNRS/INSU-IN2P3-INP (France); ESA; ASI (Italy); CNR
(Italy); INAF (Italy); NASA (USA); DoE (USA); STFC (UK); UKSA (UK); CSIC
(Spain); MINECO (Spain); RES (Spain); Tekes (Finland); AoF (Finland);
CSC (Finland); DLR (Germany); MPG (Germany); CSA (Canada); DTU Space
(Denmark); SER/SSO (Switzerland); RCN (Norway); SFI (Ireland); FCT/MCTES
(Portugal); ERC (EU); PRACE (EU); J.A. (Spain)
FX The Planck Collaboration acknowledges the support of: ESA; CNES and
CNRS/INSU-IN2P3-INP (France); ASI, CNR, and INAF (Italy); NASA and DoE
(USA); STFC and UKSA (UK); CSIC, MINECO, J.A., and RES (Spain); Tekes,
AoF, and CSC (Finland); DLR and MPG (Germany); CSA (Canada); DTU Space
(Denmark); SER/SSO (Switzerland); RCN (Norway); SFI (Ireland); FCT/MCTES
(Portugal); ERC and PRACE (EU). A description of the Planck
Collaboration and a list of its members, indicating which technical or
scientific activities they have been involved in, can be found at
http://www.cosmos.esa.int/web/planck/planck-collaboration.
NR 108
TC 2
Z9 2
U1 0
U2 0
PU EDP SCIENCES S A
PI LES ULIS CEDEX A
PA 17, AVE DU HOGGAR, PA COURTABOEUF, BP 112, F-91944 LES ULIS CEDEX A,
FRANCE
SN 1432-0746
J9 ASTRON ASTROPHYS
JI Astron. Astrophys.
PD OCT
PY 2016
VL 594
AR A22
DI 10.1051/0004-6361/201525826
PG 24
WC Astronomy & Astrophysics
SC Astronomy & Astrophysics
GA DZ4MG
UT WOS:000385832200011
ER
PT J
AU Aghanim, N
Arnaud, M
Ashdown, M
Aumont, J
Baccigalupi, C
Banday, AJ
Barreiro, RB
Bartlett, JG
Bartolo, N
Battaner, E
Benabed, K
Benoit, A
Benoit-Levy, A
Bernard, JP
Bersanelli, M
Bielewicz, P
Bock, JJ
Bonaldi, A
Bonavera, L
Bond, JR
Borrill, J
Bouchet, FR
Boulanger, F
Bucher, M
Burigana, C
Butler, RC
Calabrese, E
Cardoso, JF
Catalano, A
Challinor, A
Chiang, HC
Christensen, PR
Clements, DL
Colombo, LPL
Combet, C
Coulais, A
Crill, BP
Curto, A
Cuttaia, F
Danese, L
Davies, RD
Davis, RJ
de Bernardis, P
de Rosa, A
de Zotti, G
Delabrouille, J
Desert, FX
Di Valentino, E
Dickinson, C
Diego, JM
Dolag, K
Dole, H
Donzelli, S
Dore, O
Douspis, M
Ducout, A
Dunkley, J
Dupac, X
Efstathiou, G
Elsner, F
Ensslin, TA
Eriksen, HK
Fergusson, J
Finelli, F
Forni, O
Frailis, M
Fraisse, AA
Franceschi, E
Frejsel, A
Galeotta, S
Galli, S
Ganga, K
Gauthier, C
Gerbino, M
Giard, M
Gjerlow, E
Gonzalez-Nuevo, J
Gorski, KM
Gratton, S
Gregorio, A
Gruppuso, A
Gudmundsson, JE
Hamann, J
Hansen, FK
Harrison, DL
Helou, G
Henrot-Versille, S
Hernandez-Monteagudo, C
Herranz, D
Hildebrandt, SR
Hivon, E
Holmes, WA
Hornstrup, A
Huffenberger, KM
Hurier, G
Jaffe, AH
Jones, WC
Juvela, M
Keihanen, E
Keskitalo, R
Kiiveri, K
Knoche, J
Knox, L
Kunz, M
Kurki-Suonio, H
Lagache, G
Lahteenmaki, A
Lamarre, JM
Lasenby, A
Lattanzi, M
Lawrence, CR
Le Jeune, M
Leonardi, R
Lesgourgues, J
Levrier, F
Lewis, A
Liguori, M
Lilje, PB
Lilley, M
Linden-Vornle, M
Lindholm, V
Lopez-Caniego, M
Macias-Perez, JF
Maffei, B
Maggio, G
Maino, D
Mandolesi, N
Mangilli, A
Maris, M
Martin, PG
Martinez-Gonzalez, E
Masi, S
Matarrese, S
Meinhold, PR
Melchiorri, A
Migliaccio, M
Millea, M
Mitra, S
Miville-Deschenes, MA
Moneti, A
Montier, L
Morgante, G
Mortlock, D
Mottet, S
Munshi, D
Murphy, JA
Narimani, A
Naselsky, P
Nati, F
Natoli, P
Noviello, F
Novikov, D
Novikov, I
Oxborrow, CA
Paci, F
Pagano, L
Pajot, F
Paoletti, D
Partridge, B
Pasian, F
Patanchon, G
Pearson, TJ
Perdereau, O
Perotto, L
Pettorino, V
Piacentini, F
Piat, M
Pierpaoli, E
Pietrobon, D
Plaszczynski, S
Pointecouteau, E
Polenta, G
Ponthieu, N
Pratt, GW
Prunet, S
Puget, JL
Rachen, JP
Reinecke, M
Remazeilles, M
Renault, C
Renzi, A
Ristorcelli, I
Rocha, G
Rossetti, M
Roudier, G
d'Orfeuil, BR
Rubino-Martin, JA
Rusholme, B
Salvati, L
Sandri, M
Santos, D
Savelainen, M
Savini, G
Scott, D
Serra, P
Spencer, LD
Spinelli, M
Stolyarov, V
Stompor, R
Sunyaev, R
Sutton, D
Suur-Uski, AS
Sygnet, JF
Tauber, JA
Terenzi, L
Toffolatti, L
Tomasi, M
Tristram, M
Trombetti, T
Tucci, M
Tuovinen, J
Umana, G
Valenziano, L
Valiviita, J
Van Tent, F
Vielva, P
Villa, F
Wade, LA
Wandelt, BD
Wehus, IK
Yvon, D
Zacchei, A
Zonca, A
AF Aghanim, N.
Arnaud, M.
Ashdown, M.
Aumont, J.
Baccigalupi, C.
Banday, A. J.
Barreiro, R. B.
Bartlett, J. G.
Bartolo, N.
Battaner, E.
Benabed, K.
Benoit, A.
Benoit-Levy, A.
Bernard, J. -P.
Bersanelli, M.
Bielewicz, P.
Bock, J. J.
Bonaldi, A.
Bonavera, L.
Bond, J. R.
Borrill, J.
Bouchet, F. R.
Boulanger, F.
Bucher, M.
Burigana, C.
Butler, R. C.
Calabrese, E.
Cardoso, J. -F.
Catalano, A.
Challinor, A.
Chiang, H. C.
Christensen, P. R.
Clements, D. L.
Colombo, L. P. L.
Combet, C.
Coulais, A.
Crill, B. P.
Curto, A.
Cuttaia, F.
Danese, L.
Davies, R. D.
Davis, R. J.
de Bernardis, P.
de Rosa, A.
de Zotti, G.
Delabrouille, J.
Desert, F. -X.
Di Valentino, E.
Dickinson, C.
Diego, J. M.
Dolag, K.
Dole, H.
Donzelli, S.
Dore, O.
Douspis, M.
Ducout, A.
Dunkley, J.
Dupac, X.
Efstathiou, G.
Elsner, F.
Ensslin, T. A.
Eriksen, H. K.
Fergusson, J.
Finelli, F.
Forni, O.
Frailis, M.
Fraisse, A. A.
Franceschi, E.
Frejsel, A.
Galeotta, S.
Galli, S.
Ganga, K.
Gauthier, C.
Gerbino, M.
Giard, M.
Gjerlow, E.
Gonzalez-Nuevo, J.
Gorski, K. M.
Gratton, S.
Gregorio, A.
Gruppuso, A.
Gudmundsson, J. E.
Hamann, J.
Hansen, F. K.
Harrison, D. L.
Helou, G.
Henrot-Versille, S.
Hernandez-Monteagudo, C.
Herranz, D.
Hildebrandt, S. R.
Hivon, E.
Holmes, W. A.
Hornstrup, A.
Huffenberger, K. M.
Hurier, G.
Jaffe, A. H.
Jones, W. C.
Juvela, M.
Keihanen, E.
Keskitalo, R.
Kiiveri, K.
Knoche, J.
Knox, L.
Kunz, M.
Kurki-Suonio, H.
Lagache, G.
Lahteenmaki, A.
Lamarre, J. -M.
Lasenby, A.
Lattanzi, M.
Lawrence, C. R.
Le Jeune, M.
Leonardi, R.
Lesgourgues, J.
Levrier, F.
Lewis, A.
Liguori, M.
Lilje, P. B.
Lilley, M.
Linden-Vornle, M.
Lindholm, V.
Lopez-Caniego, M.
Macias-Perez, J. F.
Maffei, B.
Maggio, G.
Maino, D.
Mandolesi, N.
Mangilli, A.
Maris, M.
Martin, P. G.
Martinez-Gonzalez, E.
Masi, S.
Matarrese, S.
Meinhold, P. R.
Melchiorri, A.
Migliaccio, M.
Millea, M.
Mitra, S.
Miville-Deschenes, M. -A.
Moneti, A.
Montier, L.
Morgante, G.
Mortlock, D.
Mottet, S.
Munshi, D.
Murphy, J. A.
Narimani, A.
Naselsky, P.
Nati, F.
Natoli, P.
Noviello, F.
Novikov, D.
Novikov, I.
Oxborrow, C. A.
Paci, F.
Pagano, L.
Pajot, F.
Paoletti, D.
Partridge, B.
Pasian, F.
Patanchon, G.
Pearson, T. J.
Perdereau, O.
Perotto, L.
Pettorino, V.
Piacentini, F.
Piat, M.
Pierpaoli, E.
Pietrobon, D.
Plaszczynski, S.
Pointecouteau, E.
Polenta, G.
Ponthieu, N.
Pratt, G. W.
Prunet, S.
Puget, J. -L.
Rachen, J. P.
Reinecke, M.
Remazeilles, M.
Renault, C.
Renzi, A.
Ristorcelli, I.
Rocha, G.
Rossetti, M.
Roudier, G.
d'Orfeuil, B. Rouille
Rubino-Martin, J. A.
Rusholme, B.
Salvati, L.
Sandri, M.
Santos, D.
Savelainen, M.
Savini, G.
Scott, D.
Serra, P.
Spencer, L. D.
Spinelli, M.
Stolyarov, V.
Stompor, R.
Sunyaev, R.
Sutton, D.
Suur-Uski, A. -S.
Sygnet, J. -F.
Tauber, J. A.
Terenzi, L.
Toffolatti, L.
Tomasi, M.
Tristram, M.
Trombetti, T.
Tucci, M.
Tuovinen, J.
Umana, G.
Valenziano, L.
Valiviita, J.
Van Tent, F.
Vielva, P.
Villa, F.
Wade, L. A.
Wandelt, B. D.
Wehus, I. K.
Yvon, D.
Zacchei, A.
Zonca, A.
CA Planck Collaboration
TI Planck 2015 results XI. CMB power spectra, likelihoods, and robustness
of parameters
SO ASTRONOMY & ASTROPHYSICS
LA English
DT Article
DE cosmic background radiation; cosmological parameters; cosmology:
observations; methods: data analysis; methods: statistical
ID PROBE WMAP OBSERVATIONS; MICROWAVE BACKGROUND POLARIZATION; ATACAMA
COSMOLOGY TELESCOPE; SPT-SZ SURVEY; SOUTH-POLE TELESCOPE; MODE
POLARIZATION; RESOLUTION MAPS; NUMBER COUNTS; DAMPING TAIL; ANISOTROPY
AB This paper presents the Planck 2015 likelihoods, statistical descriptions of the 2-point correlation functions of the cosmic microwave background (CMB) temperature and polarization fluctuations that account for relevant uncertainties, both instrumental and astrophysical in nature. They are based on the same hybrid approach used for the previous release, i.e., a pixel-based likelihood at low multipoles (l < 30) and a Gaussian approximation to the distribution of cross-power spectra at higher multipoles. The main improvements are the use of more and better processed data and of Planck polarization information, along with more detailed models of foregrounds and instrumental uncertainties. The increased redundancy brought by more than doubling the amount of data analysed enables further consistency checks and enhanced immunity to systematic effects. It also improves the constraining power of Planck, in particular with regard to small-scale foreground properties. Progress in the modelling of foreground emission enables the retention of a larger fraction of the sky to determine the properties of the CMB, which also contributes to the enhanced precision of the spectra. Improvements in data processing and instrumental modelling further reduce uncertainties. Extensive tests establish the robustness and accuracy of the likelihood results, from temperature alone, from polarization alone, and from their combination. For temperature, we also perform a full likelihood analysis of realistic end-to-end simulations of the instrumental response to the sky, which were fed into the actual data processing pipeline; this does not reveal biases from residual low-level instrumental systematics. Even with the increase in precision and robustness, the Lambda CDM cosmological model continues to offer a very good fit to the Planck data. The slope of the primordial scalar fluctuations, n(s), is confirmed smaller than unity at more than 5 sigma from Planck alone. We further validate the robustness of the likelihood results against specific extensions to the baseline cosmology, which are particularly sensitive to data at high multipoles. For instance, the effective number of neutrino species remains compatible with the canonical value of 3.046. For this first detailed analysis of Planck polarization spectra, we concentrate at high multipoles on the E modes, leaving the analysis of the weaker B modes to future work. At low multipoles we use temperature maps at all Planck frequencies along with a subset of polarization data. These data take advantage of Planck's wide frequency coverage to improve the separation of CMB and foreground emission. Within the baseline Lambda CDM cosmology this requires tau = 0.078 +/- 0.019 for the reionization optical depth, which is significantly lower than estimates without the use of high-frequency data for explicit monitoring of dust emission. At high multipoles we detect residual systematic errors in E polarization, typically at the mu K-2 level; we therefore choose to retain temperature information alone for high multipoles as the recommended baseline, in particular for testing non-minimal models. Nevertheless, the high-multipole polarization spectra from Planck are already good enough to enable a separate high-precision determination of the parameters of the Lambda CDM model, showing consistency with those established independently from temperature information alone.
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EM bouchet@iap.fr
RI Gonzalez-Nuevo, Joaquin/I-3562-2014; Herranz, Diego/K-9143-2014;
Colombo, Loris/J-2415-2016; Lahteenmaki, Anne/L-5987-2013; Gerbino,
Martina/E-4029-2017; Barreiro, Rita Belen/N-5442-2014; bonavera,
laura/E-9368-2017;
OI TERENZI, LUCA/0000-0001-9915-6379; Valiviita, Jussi/0000-0001-6225-3693;
Toffolatti, Luigi/0000-0003-2645-7386; Lilje, Per/0000-0003-4324-7794;
Nati, Federico/0000-0002-8307-5088; Savini, Giorgio/0000-0003-4449-9416;
Pierpaoli, Elena/0000-0002-7957-8993; Juvela, Mika/0000-0002-5809-4834;
Gonzalez-Nuevo, Joaquin/0000-0003-1354-6822; Herranz,
Diego/0000-0003-4540-1417; Colombo, Loris/0000-0003-4572-7732;
Kurki-Suonio, Hannu/0000-0002-4618-3063; Zacchei,
Andrea/0000-0003-0396-1192; Stolyarov, Vladislav/0000-0001-8151-828X;
Gerbino, Martina/0000-0002-3538-1283; Barreiro, Rita
Belen/0000-0002-6139-4272; bonavera, laura/0000-0001-8039-3876;
Paoletti, Daniela/0000-0003-4761-6147
FU ESA; CNES (France); CNRS/INSU-IN2P3-INP (France); ASI (Italy); CNR
(Italy); INAF (Italy); NASA (USA); DoE (USA); STFC (UK); UKSA (UK); CSIC
(Spain); MINECO (Spain); JA (Spain); RES (Spain); Tekes (Finland); AoF
(Finland); CSC (Finland); DLR (Germany); MPG (Germany); CSA (Canada);
DTU Space (Denmark); SER/SSO (Switzerland); RCN (Norway); SFI (Ireland);
FCT/MCTES (Portugal); ERC (EU); PRACE (EU)
FX The Planck Collaboration acknowledges the support of: ESA; CNES, and
CNRS/INSU-IN2P3-INP (France); ASI, CNR, and INAF (Italy); NASA and DoE
(USA); STFC and UKSA (UK); CSIC, MINECO, JA and RES (Spain); Tekes, AoF,
and CSC (Finland); DLR and MPG (Germany); CSA (Canada); DTU Space
(Denmark); SER/SSO (Switzerland); RCN (Norway); SFI (Ireland); FCT/MCTES
(Portugal); ERC and PRACE (EU). A description of the Planck
Collaboration and a list of its members, indicating which technical or
scientific activities they have been involved in, can be found at
http://www.cosmos.esa.int/web/planck/planck-collaboration. We further
acknowledge the use of the CLASS Boltzmann code (Lesgourgues 2011) and
the Monte Python package (Audren et al. 2013) in earlier stages of this
work. The likelihood code and some of the validation work was built on
the library pmclib from the CosmoPMC package (Kilbinger et al. 2011).
This research used resources of the IN2P3 Computer Center
(http://cc.in2p3.fr) as well as of the Planck-HFI DPC infrastructure
hosted at the Institut d'Astrophysique de Paris (France) and financially
supported by CNES.
NR 148
TC 17
Z9 17
U1 0
U2 0
PU EDP SCIENCES S A
PI LES ULIS CEDEX A
PA 17, AVE DU HOGGAR, PA COURTABOEUF, BP 112, F-91944 LES ULIS CEDEX A,
FRANCE
SN 1432-0746
J9 ASTRON ASTROPHYS
JI Astron. Astrophys.
PD OCT
PY 2016
VL 594
AR A11
DI 10.1051/0004-6361/201526926
PG 99
WC Astronomy & Astrophysics
SC Astronomy & Astrophysics
GA DZ4MG
UT WOS:000385832200026
ER
PT J
AU Aliu, E
Archambault, S
Archer, A
Arlen, T
Aune, T
Barnacka, A
Behera, B
Beilicke, M
Benbow, W
Berger, K
Bird, R
Bottcher, M
Bouvier, A
Buchovecky, M
Buckley, JH
Bugaev, V
Cardenzana, JV
Cerruti, M
Cesarini, A
Chen, X
Ciupik, L
Collins-Hughes, E
Connolly, MP
Cui, W
Dumm, J
Eisch, JD
Falcone, A
Federici, S
Feng, Q
Finley, JP
Fleischhack, H
Fortin, P
Fortson, L
Furniss, A
Galante, N
Gall, D
Gillanders, GH
Griffin, S
Griffiths, ST
Grube, J
Gyuk, G
Hutten, M
Hakansson, N
Holder, J
Hughes, G
Humensky, TB
Johnson, CA
Kaaret, P
Kar, P
Kelley-Hoskins, N
Kertzman, M
Khassen, Y
Kieda, D
Krause, M
Krawczynski, H
Krennrich, F
Lang, MJ
Madhavan, AS
Maier, G
McArthur, S
McCann, A
Meagher, K
Millis, J
Moriarty, P
Mukherjee, R
Nieto, D
de Bhroithe, AO
Ong, RA
Orr, M
Otte, AN
Pandel, D
Park, N
Pelassa, V
Perkins, JS
Pichel, A
Pohl, M
Popkow, A
Quinn, J
Ragan, K
Reyes, LC
Reynolds, PT
Roache, E
Rousselle, J
Rovero, AC
Saxon, DB
Sembroski, GH
Shahinyan, K
Sheidaei, F
Skole, C
Smith, AW
Staszak, D
Telezhinsky, I
Theiling, M
Todd, NW
Tucci, JV
Tyler, J
Varlotta, A
Vassiliev, VV
Vincent, S
Wakely, SP
Weiner, OM
Weinstein, A
Welsing, R
Wilhelm, A
Williams, DA
Zitzer, B
Baring, MG
Gonzalez, JB
Cillis, AN
Horan, D
Paneque, D
AF Aliu, E.
Archambault, S.
Archer, A.
Arlen, T.
Aune, T.
Barnacka, A.
Behera, B.
Beilicke, M.
Benbow, W.
Berger, K.
Bird, R.
Bottcher, M.
Bouvier, A.
Buchovecky, M.
Buckley, J. H.
Bugaev, V.
Cardenzana, J. V.
Cerruti, M.
Cesarini, A.
Chen, X.
Ciupik, L.
Collins-Hughes, E.
Connolly, M. P.
Cui, W.
Dumm, J.
Eisch, J. D.
Falcone, A.
Federici, S.
Feng, Q.
Finley, J. P.
Fleischhack, H.
Fortin, P.
Fortson, L.
Furniss, A.
Galante, N.
Gall, D.
Gillanders, G. H.
Griffin, S.
Griffiths, S. T.
Grube, J.
Gyuk, G.
Huetten, M.
Hakansson, N.
Holder, J.
Hughes, G.
Humensky, T. B.
Johnson, C. A.
Kaaret, P.
Kar, P.
Kelley-Hoskins, N.
Kertzman, M.
Khassen, Y.
Kieda, D.
Krause, M.
Krawczynski, H.
Krennrich, F.
Lang, M. J.
Madhavan, A. S.
Maier, G.
McArthur, S.
McCann, A.
Meagher, K.
Millis, J.
Moriarty, P.
Mukherjee, R.
Nieto, D.
de Bhroithe, A. O'Faolain
Ong, R. A.
Orr, M.
Otte, A. N.
Pandel, D.
Park, N.
Pelassa, V.
Perkins, J. S.
Pichel, A.
Pohl, M.
Popkow, A.
Quinn, J.
Ragan, K.
Reyes, L. C.
Reynolds, P. T.
Roache, E.
Rousselle, J.
Rovero, A. C.
Saxon, D. B.
Sembroski, G. H.
Shahinyan, K.
Sheidaei, F.
Skole, C.
Smith, A. W.
Staszak, D.
Telezhinsky, I.
Theiling, M.
Todd, N. W.
Tucci, J. V.
Tyler, J.
Varlotta, A.
Vassiliev, V. V.
Vincent, S.
Wakely, S. P.
Weiner, O. M.
Weinstein, A.
Welsing, R.
Wilhelm, A.
Williams, D. A.
Zitzer, B.
Baring, M. G.
Gonzalez, J. Becerra
Cillis, A. N.
Horan, D.
Paneque, D.
CA Veritas Collaboration
TI Very high energy outburst of Markarian 501 in May 2009
SO ASTRONOMY & ASTROPHYSICS
LA English
DT Article
DE BL Lacertae objects: individual: Mrk 501; gamma rays: galaxies
ID BL-LACERTAE OBJECTS; LARGE-AREA TELESCOPE; GAMMA-RAY EMISSION; OPTICAL
POLARIZATION PROPERTIES; EXTRAGALACTIC RADIO-SOURCES; ACTIVE GALACTIC
NUCLEI; X-RAY; MULTIWAVELENGTH OBSERVATIONS; SPECTRAL VARIABILITY;
INTERNAL SHOCKS
AB The very high energy (VHE; E > 100 GeV) blazar Markarian 501 was observed between April 17 and May 5 (MJD 54 938-54 956), 2009, as part of an extensive multiwavelength campaign from radio to VHE. Strong VHE yray activity was detected on May 1st with Whipple and VERITAS, when the flux (E > 400 GeV) increased to 10 times the preflare baseline flux (3.9 x 10(-11) ph cm(-2) s(-1)), reaching five times the flux of the Crab Nebula. This coincided with a decrease in the optical polarization and a rotation of the polarization angle by 15. This VHE flare showed a fast flux variation with an increase of a factor similar to 4 in 25 min, and a falling time of similar to 50 min. We present the observations of the quiescent state previous to the flare and of the high state after the flare, focusing on the flux and spectral variability from Whipple, VERITAS, Fermi-LAT, RXTE, and Swift combined with optical and radio data.
C1 [Aliu, E.; Mukherjee, R.] Columbia Univ, Barnard Coll, Dept Phys & Astron, New York, NY 10027 USA.
[Archambault, S.; Griffin, S.; McCann, A.; Ragan, K.; Tyler, J.] McGill Univ, Dept Phys, Montreal, PQ H3A 2T8, Canada.
[Archer, A.; Beilicke, M.; Buckley, J. H.; Bugaev, V.; Krawczynski, H.; Todd, N. W.] Washington Univ, Dept Phys, St Louis, MO 63130 USA.
[Arlen, T.; Aune, T.; Buchovecky, M.; Ong, R. A.; Popkow, A.; Rousselle, J.; Vassiliev, V. V.] Univ Calif Los Angeles, Dept Phys & Astron, Los Angeles, CA 90095 USA.
[Barnacka, A.] Harvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA.
[Behera, B.; Chen, X.; Federici, S.; Fleischhack, H.; Huetten, M.; Hughes, G.; Kelley-Hoskins, N.; Krause, M.; Maier, G.; de Bhroithe, A. O'Faolain; Pohl, M.; Skole, C.; Telezhinsky, I.; Vincent, S.; Welsing, R.; Wilhelm, A.] DESY, Platanenallee 6, D-15738 Zeuthen, Germany.
[Benbow, W.; Cerruti, M.; Fortin, P.; Galante, N.; Pelassa, V.; Roache, E.] Harvard Smithsonian Ctr Astrophys, Fred Lawrence Whipple Observ, Amado, AZ 85645 USA.
[Berger, K.; Holder, J.; Saxon, D. B.] Univ Delaware, Dept Phys & Astron, Newark, DE 19716 USA.
[Berger, K.; Holder, J.; Saxon, D. B.] Univ Delaware, Bartol Res Inst, Newark, DE 19716 USA.
[Bird, R.; Collins-Hughes, E.; Khassen, Y.; Quinn, J.] Univ Coll Dublin, Sch Phys, Dublin 4, Ireland.
[Bottcher, M.] North West Univ, Ctr Space Res, Private Bag X6001, ZA-2520 Potchefstroom, South Africa.
[Bouvier, A.; Johnson, C. A.; Williams, D. A.] Univ Calif Santa Cruz, Santa Cruz Inst Particle Phys, Santa Cruz, CA 95064 USA.
[Bouvier, A.; Johnson, C. A.; Williams, D. A.] Univ Calif Santa Cruz, Dept Phys, Santa Cruz, CA 95064 USA.
[Cardenzana, J. V.; Eisch, J. D.; Krennrich, F.; Madhavan, A. S.; Orr, M.; Weinstein, A.] Iowa State Univ, Dept Phys & Astron, Ames, IA 50011 USA.
[Cesarini, A.; Connolly, M. P.; Gillanders, G. H.; Lang, M. J.; Moriarty, P.] Natl Univ Ireland Galway, Sch Phys, Univ Rd, Galway, Ireland.
[Chen, X.; Federici, S.; Hakansson, N.; Pohl, M.; Telezhinsky, I.; Wilhelm, A.] Univ Potsdam, Inst Phys & Astron, D-14476 Potsdam, Germany.
[Ciupik, L.; Grube, J.; Gyuk, G.] Adler Planetarium & Astron Museum, Dept Astron, Chicago, IL 60605 USA.
[Cui, W.; Feng, Q.; Finley, J. P.; McArthur, S.; Sembroski, G. H.; Theiling, M.; Tucci, J. V.; Varlotta, A.] Purdue Univ, Dept Phys & Astron, W Lafayette, IN 47907 USA.
[Dumm, J.; Fortson, L.; Shahinyan, K.] Univ Minnesota, Sch Phys & Astron, Minneapolis, MN 55455 USA.
[Falcone, A.] Penn State Univ, Dept Astron & Astrophys, Davey Lab 525, University Pk, PA 16802 USA.
[Furniss, A.] Calif State Univ East Bay, Dept Phys, Hayward, CA 94542 USA.
[Gall, D.; Griffiths, S. T.; Kaaret, P.] Univ Iowa, Dept Phys & Astron, Van Allen Hall, Iowa City, IA 52242 USA.
[Humensky, T. B.; Nieto, D.; Weiner, O. M.] Columbia Univ, Dept Phys, New York, NY 10027 USA.
[Kar, P.; Kieda, D.; Sheidaei, F.] Univ Utah, Dept Phys & Astron, Salt Lake City, UT 84112 USA.
[Kertzman, M.] Depauw Univ, Dept Phys & Astron, Greencastle, IN 46135 USA.
[Meagher, K.; Otte, A. N.] Georgia Inst Technol, Sch Phys, 837 State St NW, Atlanta, GA 30332 USA.
[Meagher, K.; Otte, A. N.] Georgia Inst Technol, Ctr Relativist Astrophys, 837 State St NW, Atlanta, GA 30332 USA.
[Millis, J.] Anderson Univ, Dept Phys, 1100 East 5th St, Anderson, IN 46012 USA.
[Moriarty, P.] Galway Mayo Inst Technol, Dept Life & Phys Sci, Dublin Rd, Galway, Ireland.
[Pandel, D.] Grand Valley State Univ, Dept Phys, Allendale, MI 49401 USA.
[Park, N.; Staszak, D.; Wakely, S. P.] Univ Chicago, Enrico Fermi Inst, Chicago, IL 60637 USA.
[Perkins, J. S.; Gonzalez, J. Becerra; Cillis, A. N.] NASA, Goddard Space Flight Ctr, Code 661, Greenbelt, MD 20771 USA.
[Pichel, A.; Rovero, A. C.; Cillis, A. N.] Inst Astron & Fis Espacio, Casilla Correo 67,Sucursal 28,C1428ZAA, Buenos Aires, DF, Argentina.
[Reyes, L. C.] Calif Polytech State Univ San Luis Obispo, Dept Phys, San Luis Obispo, CA 94307 USA.
[Reynolds, P. T.] Cork Inst Technol, Dept Phys Sci, Cork, Ireland.
[Smith, A. W.] Argonne Natl Lab, 9700 S Cass Ave, Argonne, IL 60439 USA.
[Zitzer, B.] Univ Maryland, College Pk, MD 20742 USA.
[Zitzer, B.] NASA, GSFC, College Pk, MD 20742 USA.
[Baring, M. G.] Rice Univ, Dept Phys & Astron, POB 1892, Houston, TX 77251 USA.
[Gonzalez, J. Becerra] Univ Maryland, Dept Phys, College Pk, MD 20742 USA.
[Gonzalez, J. Becerra] Univ Maryland, Dept Astron, College Pk, MD 20742 USA.
[Horan, D.] Ecole Polytech, CNRS, IN2P3, Lab Leprince Ringuet, F-91128 Palaiseau, France.
[Paneque, D.] Stanford Univ, Dept Phys, Kavli Inst Particle Astrophys & Cosmol, WW Hansen Expt Phys Lab, Stanford, CA 94305 USA.
[Paneque, D.] Stanford Univ, SLAC Natl Accelerator Lab, Stanford, CA 94305 USA.
[Paneque, D.] Max Planck Inst Phys & Astrophys, D-80805 Munich, Germany.
RP Pichel, A (reprint author), Inst Astron & Fis Espacio, Casilla Correo 67,Sucursal 28,C1428ZAA, Buenos Aires, DF, Argentina.
EM anapichel@iafe.uba.ar
OI Pandel, Dirk/0000-0003-2085-5586; Krause, Maria/0000-0001-7595-0914
FU US Department of Energy Office of Science; US National Science
Foundation; Smithsonian Institution; NSERC in Canada; South African
Research Chairs Initiative (SARChI) by National Research Foundation;
Department of Science and Technology of South Africa
FX This research is supported by grants from the US Department of Energy
Office of Science, the US National Science Foundation and the
Smithsonian Institution, and by NSERC in Canada. We acknowledge the
excellent work of the technical support staff at the Fred Lawrence
Whipple Observatory and at the collaborating institutions in the
construction and operation of the instrument. The VERITAS Collaboration
is grateful to Trevor Weekes for his seminal contributions and
leadership in the field of VHE gamma-ray astrophysics, which made this
study possible. The Fermi LAT Collaboration acknowledges support from a
number of agencies and institutes for both development and the operation
of the LAT as well as scientific data analysis. These include NASA and
DOE in the United States, CEA/Irfu and IN2P3/CNRS in France, ASI and
INFN in Italy, MEXT, KEK, and JAXA in Japan, and the K. A. Wallenberg
Foundation, the Swedish Research Council and the National Space Board in
Sweden. Additional support from INAF in Italy and CNES in France for
science analysis during the operations phase is also gratefully
acknowledged. M.B. acknowledges support through the South African
Research Chairs Initiative (SARChI) by the National Research Foundation
and the Department of Science and Technology of South Africa.
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SC Astronomy & Astrophysics
GA DZ4MG
UT WOS:000385832200085
ER
PT J
AU Belczynski, K
Heger, A
Gladysz, W
Ruiter, AJ
Woosley, S
Wiktorowicz, G
Chen, HY
Bulik, T
O'Shaughnessy, R
Holz, DE
Fryer, CL
Berti, E
AF Belczynski, K.
Heger, A.
Gladysz, W.
Ruiter, A. J.
Woosley, S.
Wiktorowicz, G.
Chen, H. -Y.
Bulik, T.
O'Shaughnessy, R.
Holz, D. E.
Fryer, C. L.
Berti, E.
TI The effect of pair-instability mass loss on black-hole mergers
SO ASTRONOMY & ASTROPHYSICS
LA English
DT Article
DE stars: massive; black hole physics; gravitational waves
ID M-CIRCLE-DOT; GRAVITATIONAL-WAVE DETECTION; STAR-FORMATION RATE;
GAMMA-RAY BURSTS; COMMON ENVELOPE; NEUTRON-STARS; EXPLOSION MECHANISM;
STELLAR EVOLUTION; COMPACT OBJECTS; POPULATION III
AB Context. Mergers of two stellar-origin black holes are a prime source of gravitational waves and are under intensive investigation. One crucial ingredient in their modeling has been neglected: pair-instability pulsation supernovae with associated severe mass loss may suppress the formation of massive black holes, decreasing black-hole-merger rates for the highest black-hole masses.
Aims. We demonstrate the effects of pair-instability pulsation supernovae on merger rate and mass using populations of double black-hole binaries formed through the isolated binary classical evolution channel.
Methods. The mass loss from pair-instability pulsation supernova is estimated based on existing hydrodynamical calculations. This mass loss is incorporated into the StarTrack population synthesis code. StarTrack is used to generate double black-hole populations with and without pair-instability pulsation supernova mass loss.
Results. The mass loss associated with pair-instability pulsation supernovae limits the Population I/II stellar-origin black-hole mass to 50 M-circle dot, in tension with earlier predictions that the maximum black-hole mass could be as high as 100 M-circle dot. In our model, neutron stars form with mass 1 2 M-circle dot. We then encounter the first mass gap at 2 5 M-circle dot with the compact object absence due to rapid supernova explosions, followed by the formation of black holes with mass 5 50 M-circle dot, with a second mass gap at 50 135 M-circle dot created by pair-instability pulsation supernovae and by pair-instability supernovae. Finally, black holes with masses above 135 M-circle dot may potentially form to arbitrarily high mass limited only by the extent of the initial mass function and the strength of stellar winds. Suppression of double black-hole-merger rates by pair-instability pulsation supernovae is negligible for our evolutionary channel. Our standard evolutionary model, with the inclusion of pair-instability pulsation supernovae and pair-instability supernovae, is fully consistent with the Laser Interferometric Gravitational-wave Observatory (LIGO) observations of black-hole mergers: GW150914, GW151226, and LVT151012. The LIGO results are inconsistent with high (greater than or similar to 400 km s(-1)) black hole (BH) natal kicks. We predict the detection of several, and up to as many as similar to 60, BH-BH mergers with a total mass of 10 150 M-circle dot (most likely range: 20 80 M-circle dot) in the forthcoming similar to 60 effective days of the LIGO O2 observations, assuming the detectors reach the optimistic target O2 sensitivity.
C1 [Belczynski, K.; Gladysz, W.; Wiktorowicz, G.; Bulik, T.] Warsaw Univ, Astron Observ, Ujazdowskie 4, PL-00478 Warsaw, Poland.
[Heger, A.] Monash Univ, Monash Ctr Astrophys, Sch Phys & Astron, Clayton, Vic 3800, Australia.
[Heger, A.] Univ Minnesota, Sch Phys & Astron, Minneapolis, MN 55455 USA.
[Heger, A.] Shanghai Jiao Tong Univ, Ctr Nucl Astrophys, Dept Phys & Astron, Shanghai 200240, Peoples R China.
[Heger, A.] Michigan State Univ, Joint Inst Nucl Astrophys, Natl Superconducting Cyclotron Lab, Cyclotron Lab 1, E Lansing, MI 48824 USA.
[Ruiter, A. J.] Australian Natl Univ, Res Sch Astron & Astrophys, Canberra, ACT 2611, Australia.
[Ruiter, A. J.] ARC Ctr Excellence All Sky Astrophys CAASTRO, Sydney, NSW 2006, Australia.
[Woosley, S.] Univ Calif Santa Cruz, Dept Astron & Astrophys, Santa Cruz, CA 95064 USA.
[Chen, H. -Y.; Holz, D. E.] Univ Chicago, Enrico Fermi Inst, Dept Phys, Dept Astron & Astrophys, Chicago, IL 60637 USA.
[Chen, H. -Y.; Holz, D. E.] Univ Chicago, Kavli Inst Cosmol Phys, Chicago, IL 60637 USA.
[O'Shaughnessy, R.] Rochester Inst Technol, Ctr Computat Relat & Gravitat, Rochester, NY 14623 USA.
[Fryer, C. L.] Los Alamos Natl Lab, CCS-2,MSD409, Los Alamos, NM 87545 USA.
[Berti, E.] Univ Mississippi, Dept Phys & Astron, University, MS 38677 USA.
[Berti, E.] Univ Lisbon, Inst Super Tecn, CENTRA, Dept Fis, Ave Rovisco Pais 1, P-1049 Lisbon, Portugal.
RP Belczynski, K (reprint author), Warsaw Univ, Astron Observ, Ujazdowskie 4, PL-00478 Warsaw, Poland.
EM chrisbelczynski@gmail.com
OI Berti, Emanuele/0000-0003-0751-5130
FU NCN grant Sonata Bis 2 [Dec-2012/07/E/ST9/01360]; NCN grant OPUS
[2015/19/B/ST9/01099]; Australian Research Council Centre of Excellence
for All-sky Astrophysics (CAASTRO) [CE110001020]; CAASTRO; Stromlo
Distinguished Visitor Program at the Research School of Astronomy and
Astrophysics, Australian National University, Canberra; Australian
Research Council through an ARC Future Fellowship [FT120100363]; US
National Science Foundation [PHY-1430152]; NCN
[UMO-2014/15/Z/ST9/00038]; NSF [PHY 1505629, AST 1412449]; NSF CAREER
grant [PHY-1151836, PHY-1055103]; Kavli Institute for Cosmological
Physics at the University of Chicago through NSF [PHY-1125897]; FCT
under the IF2014 Programme [IF/00797/2014/CP1214/CT0012];
[H2020-MSCA-RISE-2015]; [StronGrHEP-690904]
FX We would like to thank Sung-Chul Yoon, Mirek Giersz, and John Beacom for
very useful discussions on the subject of this study. We would like to
thank thousands of Universe@home users that have provided their personal
computers and phones for our simulations, and in particular to Krzysztof
Piszczek (program IT manager). K.B. acknowledges support from the NCN
grant Sonata Bis 2 (Dec-2012/07/E/ST9/01360) and the NCN grant OPUS
(2015/19/B/ST9/01099). AJR is funded by the Australian Research Council
Centre of Excellence for All-sky Astrophysics (CAASTRO) through Grant
No. CE110001020. K.B. is thankful for support from CAASTRO and the
Stromlo Distinguished Visitor Program at the Research School of
Astronomy and Astrophysics, Australian National University, Canberra.
A.H. acknowledges support by the Australian Research Council through an
ARC Future Fellowship FT120100363 and by the US National Science
Foundation under Grant No. PHY-1430152 (JINA Center for the Evolution of
the Elements). T.B. is grateful for support by the NCN grant
UMO-2014/15/Z/ST9/00038. R.O. acknowledges support from Grants: NSF PHY
1505629 and (via subcontract) AST 1412449. D.E.H. was supported by NSF
CAREER grant PHY-1151836. He also acknowledges support from the Kavli
Institute for Cosmological Physics at the University of Chicago through
NSF grant PHY-1125897 as well as an endowment from the Kavli Foundation.
E.B. was supported by NSF CAREER grant PHY-1055103 and by FCT contract
IF/00797/2014/CP1214/CT0012 under the IF2014 Programme. This work was
supported by the H2020-MSCA-RISE-2015 Grant No. StronGrHEP-690904.
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SC Astronomy & Astrophysics
GA DZ4MG
UT WOS:000385832200104
ER
PT J
AU Galicher, R
Marois, C
Macintosh, B
Zuckerman, B
Barman, T
Konopacky, Q
Song, I
Patience, J
Lafreniere, D
Doyon, R
Nielsen, EL
AF Galicher, R.
Marois, C.
Macintosh, B.
Zuckerman, B.
Barman, T.
Konopacky, Q.
Song, I.
Patience, J.
Lafreniere, D.
Doyon, R.
Nielsen, E. L.
TI The International Deep Planet Survey II. The frequency of directly
imaged giant exoplanets with stellar mass
SO ASTRONOMY & ASTROPHYSICS
LA English
DT Article
DE planets and satellites: gaseous planets; planets and satellites:
fundamental parameters; methods: observational; methods: data analysis;
methods: statistical; instrumentation: high angular resolution
ID SUN-LIKE STARS; FINDING CAMPAIGN DISCOVERY; GENEVA-COPENHAGEN SURVEY;
ADAPTIVE OPTICS SYSTEM; PICTORIS MOVING GROUP; MAIN-SEQUENCE STARS;
VISUAL DOUBLE STARS; DUSTY DEBRIS DISKS; A-TYPE STARS; YOUNG STARS
AB Context. Radial velocity and transit methods are effective for the study of short orbital period exoplanets but they hardly probe objects at large separations for which direct imaging can be used.
Aims. We carried out the international deep planet survey of 292 young nearby stars to search for giant exoplanets and determine their frequency.
Methods. We developed a pipeline for a uniform processing of all the data that we have recorded with NIRC2/Keck II, NIRI/Gemini North, NICI/Gemini South, and NACO/VLT for 14 yr. The pipeline first applies cosmetic corrections and then reduces the speckle intensity to enhance the contrast in the images.
Results. The main result of the international deep planet survey is the discovery of the HR8799 exoplanets. We also detected 59 visual multiple systems including 16 new binary stars and 2 new triple stellar systems, as well as 2279 point-like sources. We used Monte Carlo simulations and the Bayesian theorem to determine that 1.05(-0.70)(+2.80)% of stars harbor at least one giant planet between 0.5 and 14 MJ and between 20 and 300AU. This result is obtained assuming uniform distributions of planet masses and semi-major axes. If we consider power law distributions as measured for close-in planets instead, the derived frequency is 2.30(-1.55)(+5.95)%, recalling the strong impact of assumptions on Monte Carlo output distributions. We also find no evidence that the derived frequency depends on the mass of the hosting star, whereas it does for close-in planets.
Conclusions. The international deep planet survey provides a database of confirmed background sources that may be useful for other exoplanet direct imaging surveys. It also puts new constraints on the number of stars with at least one giant planet reducing by a factor of two the frequencies derived by almost all previous works.
C1 [Galicher, R.] Univ Paris 06, Univ Paris Diderot, CNRS, Observ Paris,LESIA, 5 Pl Jules Janssen, F-92190 Meudon, France.
[Galicher, R.] CNRS, Observ Paris, Grp Interet Sci PHASE Partenariat Haute Reslout A, F-75000 Paris, France.
[Galicher, R.] Univ Paris Diderot, F-75000 Paris, France.
[Galicher, R.; Marois, C.] Natl Res Council Canada, 5071 W Saanich Rd, Victoria, BC V9E 2E7, Canada.
[Marois, C.; Macintosh, B.] Lawrence Livermore Natl Lab, 7000 East Ave, Livermore, CA 94550 USA.
[Macintosh, B.; Nielsen, E. L.] Stanford Univ, Kavli Inst Particle Astrophys & Cosmol, Stanford, CA 94305 USA.
[Zuckerman, B.] Univ Calif Los Angeles, Dept Phys & Astron, Los Angeles, CA 90095 USA.
[Barman, T.] Univ Arizona, Lunar & Planetary Lab, Tucson, AZ 85721 USA.
[Konopacky, Q.] Univ Calif San Diego, CASS, La Jolla, CA 92093 USA.
[Song, I.] Univ Georgia, Dept Phys & Astron, Athens, GA 30602 USA.
[Patience, J.] Arizona State Univ, Tempe, AZ 85281 USA.
[Lafreniere, D.; Doyon, R.] Univ Montreal, Dept Phys, 6128 Succ Ctr Ville, Montreal, PQ H3C 3J7, Canada.
[Nielsen, E. L.] SETI Inst, Carl Sagan Ctr, 189 Bernardo Ave, Mountain View, CA 94043 USA.
RP Galicher, R (reprint author), Univ Paris 06, Univ Paris Diderot, CNRS, Observ Paris,LESIA, 5 Pl Jules Janssen, F-92190 Meudon, France.; Galicher, R (reprint author), CNRS, Observ Paris, Grp Interet Sci PHASE Partenariat Haute Reslout A, F-75000 Paris, France.; Galicher, R (reprint author), Univ Paris Diderot, F-75000 Paris, France.; Galicher, R (reprint author), Natl Res Council Canada, 5071 W Saanich Rd, Victoria, BC V9E 2E7, Canada.
EM raphael.galicher@obspm.fr
FU W. M. Keck Foundation
FX The authors acknowledge the referee for constructive comments and
suggestions. The authors wish to recognize and acknowledge the very
significant cultural role and reverence that the summit of Mauna Kea has
always had within the indigenous Hawaiian community. We are most
fortunate to have the opportunity to conduct observations from this
mountain. This research has made use of the SIMBAD database, operated at
CDS, Strasbourg, France (Wenger et al. 2000). Some of the data presented
herein were obtained at the W. M. Keck Observatory, which is operated as
a scientific partnership among the California Institute of Technology,
the University of California, and the National Aeronautics and Space
Administration. The Observatory was made possible by the generous
financial support of the W. M. Keck Foundation. This research has made
use of the Keck Observatory Archive (KOA), which is operated by the W.
M. Keck Observatory and the NASA Exoplanet Science Institute (NExScI),
under contract with the National Aeronautics and Space Administration.
Based on observations obtained at the Gemini Observatory (acquired
through the Gemini Observatory Archive and the Gemini Science Archive),
which is operated by the Association of Universities for Research in
Astronomy, Inc., under a cooperative agreement with the NSF on behalf of
the Gemini partnership: the National Science Foundation (United States),
the National Research Council (Canada), CONICYT (Chile), Ministerio de
Ciencia, Tecnologia e Innovacion Productiva (Argentina), and Ministerio
da Ciencia, Tecnologia e Inovacao (Brazil).
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PT J
AU Hoen, B
Atkinson-Palombo, C
AF Hoen, Ben
Atkinson-Palombo, Carol
TI Wind Turbines, Amenities and Disamenities: A Study of Home Value Impacts
in Densely Populated Massachusetts
SO JOURNAL OF REAL ESTATE RESEARCH
LA English
DT Article
ID RESIDENTIAL PROPERTY-VALUES; HOUSE PRICES; OPEN SPACE; NOISE;
REGRESSION; POWER
AB In this study, we investigate the effect of planned or operating wind turbines on urban home values. Previous studies, which largely produced non-significant findings, focused on rural settings. We analyzed more than 122,000 home sales, between 1998 and 2012, that occurred near 41 turbines in densely populated Massachusetts communities. Although we found the effects from various negative features (such as electricity transmission lines) and positive features (such as open space) generally accorded with previous studies, we found no net effects due to turbines in these communities. We also found no unique impact on the rate of home sales near wind turbines.
C1 [Hoen, Ben] Lawrence Berkeley Natl Lab, Berkeley, CA 94720 USA.
[Atkinson-Palombo, Carol] Univ Connecticut, Storrs, CT 06269 USA.
RP Hoen, B (reprint author), Lawrence Berkeley Natl Lab, Berkeley, CA 94720 USA.
EM bhoen@lbl.gov; carol.atkinson-palombo@uconn.edu
FU Massachusetts Clean Energy Center; Office of Energy Efficiency and
Renewable Energy (Wind and Water Power Technologies Office) of the U.S.
Department of Energy [DE-AC02-05CH1123]
FX This work was supported in part by the Massachusetts Clean Energy Center
and the Office of Energy Efficiency and Renewable Energy (Wind and Water
Power Technologies Office) of the U.S. Department of Energy under
Contract No. DE-AC02-05CH1123. We thank the anonymous reviewers for
their insightful comments. A previous version of this paper received the
Marc Louargand Award for the Best Research Paper by a Practicing Real
Estate Professional presented at the 2014 ARES Annual Meeting.
NR 51
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U1 6
U2 6
PU AMER REAL ESTATE SOC
PI CLEMSON
PA CLEMSON UNIV, SCH BUSINESS & BEHAVIORAL SCI, DEPT FINANCE, 314 SIRRINE
HALL, CLEMSON, SC 29634 USA
SN 0896-5803
J9 J REAL ESTATE RES
JI J. Real Estate Res.
PD OCT-DEC
PY 2016
VL 38
IS 4
BP 473
EP 504
PG 32
WC Business, Finance; Economics
SC Business & Economics
GA EH8UD
UT WOS:000392046900001
ER
PT J
AU Kennel, SJ
Williams, A
Martin, EB
Richey, T
Stuckey, A
Macy, S
Cheng, X
Wall, JS
AF Kennel, S. J.
Williams, A.
Martin, E. B.
Richey, T.
Stuckey, A.
Macy, S.
Cheng, X.
Wall, J. S.
TI Preclinical validation of synthetic peptide p5 plus 14 as a
multi-platform molecular imaging agent for systemic amyloidosis
SO EUROPEAN JOURNAL OF NUCLEAR MEDICINE AND MOLECULAR IMAGING
LA English
DT Meeting Abstract
CT Annual Congress of the European-Association-of-Nuclear-Medicine (EANM)
CY OCT 15-19, 2016
CL Barcelona, SPAIN
SP European Assoc Nucl Med
C1 [Kennel, S. J.; Williams, A.; Martin, E. B.; Richey, T.; Stuckey, A.; Macy, S.; Wall, J. S.] UT GSM, Knoxville, TN USA.
[Cheng, X.] Oak Ridge Natl Lab, Oak Ridge, TN USA.
NR 0
TC 0
Z9 0
U1 0
U2 0
PU SPRINGER
PI NEW YORK
PA 233 SPRING ST, NEW YORK, NY 10013 USA
SN 1619-7070
EI 1619-7089
J9 EUR J NUCL MED MOL I
JI Eur. J. Nucl. Med. Mol. Imaging
PD OCT
PY 2016
VL 43
SU 1
MA EPW59
BP S229
EP S229
PG 1
WC Radiology, Nuclear Medicine & Medical Imaging
SC Radiology, Nuclear Medicine & Medical Imaging
GA EH5GW
UT WOS:000391801600572
ER
PT J
AU Mirzadeh, S
Rojas, JV
McLaughlin, MF
Woodward, JD
Robertson, D
Kennel, S
AF Mirzadeh, S.
Rojas, J. V.
McLaughlin, M. F.
Woodward, J. D.
Robertson, D.
Kennel, S.
TI Lanthanum phosphate nanoparticles as carriers for Ac-225, Ra-223 &
Ra-225 for targeted alpha therapy
SO EUROPEAN JOURNAL OF NUCLEAR MEDICINE AND MOLECULAR IMAGING
LA English
DT Meeting Abstract
CT Annual Congress of the European-Association-of-Nuclear-Medicine (EANM)
CY OCT 15-19, 2016
CL Barcelona, SPAIN
SP European Assoc Nucl Med
C1 [Mirzadeh, S.; Woodward, J. D.] Oak Ridge Natl Lab, Med Radioisotope Program, Oak Ridge, TN USA.
[Rojas, J. V.] Virginia Commonwealth Univ, Dept Mech & Nucl Engn, Richmond, VA USA.
[McLaughlin, M. F.; Robertson, D.] Univ Missouri, Dept Chem, Columbia, MO 65211 USA.
[McLaughlin, M. F.; Robertson, D.] Univ Missouri, Res Reactor, Columbia, MO USA.
[Kennel, S.] Univ TN, Grad Sch Med, Knoxville, TN USA.
NR 0
TC 0
Z9 0
U1 0
U2 0
PU SPRINGER
PI NEW YORK
PA 233 SPRING ST, NEW YORK, NY 10013 USA
SN 1619-7070
EI 1619-7089
J9 EUR J NUCL MED MOL I
JI Eur. J. Nucl. Med. Mol. Imaging
PD OCT
PY 2016
VL 43
SU 1
MA OP674
BP S199
EP S200
PG 2
WC Radiology, Nuclear Medicine & Medical Imaging
SC Radiology, Nuclear Medicine & Medical Imaging
GA EH5GW
UT WOS:000391801600492
ER
PT J
AU Pruszynski, M
Cedrowska, E
Radchenko, V
John, KD
Bruchertseifer, F
Morgenstern, A
D'Huyvetter, M
Lahoutte, T
AF Pruszynski, M.
Cedrowska, E.
Radchenko, V.
John, K. D.
Bruchertseifer, F.
Morgenstern, A.
D'Huyvetter, M.
Lahoutte, T.
TI Anti HER2 Nanobody Labeled with Ac-225 as a Potential
Radiopharmaceutical for TRT
SO EUROPEAN JOURNAL OF NUCLEAR MEDICINE AND MOLECULAR IMAGING
LA English
DT Meeting Abstract
CT Annual Congress of the European-Association-of-Nuclear-Medicine (EANM)
CY OCT 15-19, 2016
CL Barcelona, SPAIN
SP European Assoc Nucl Med
C1 [Pruszynski, M.; Cedrowska, E.] Inst Nucl Chem & Technol, Warsaw, Poland.
[Radchenko, V.; John, K. D.] Los Alamos Natl Lab, Los Alamos, NM USA.
[Bruchertseifer, F.; Morgenstern, A.] Inst Transuranium Elements, Joint Res Ctr, Karlsruhe, Germany.
[D'Huyvetter, M.; Lahoutte, T.] Vrije Univ Brussel, Brussels, Belgium.
NR 0
TC 0
Z9 0
U1 1
U2 1
PU SPRINGER
PI NEW YORK
PA 233 SPRING ST, NEW YORK, NY 10013 USA
SN 1619-7070
EI 1619-7089
J9 EUR J NUCL MED MOL I
JI Eur. J. Nucl. Med. Mol. Imaging
PD OCT
PY 2016
VL 43
SU 1
MA OP590
BP S177
EP S177
PG 1
WC Radiology, Nuclear Medicine & Medical Imaging
SC Radiology, Nuclear Medicine & Medical Imaging
GA EH5GW
UT WOS:000391801600437
ER
PT J
AU John, KD
AF John, K. D.
TI US DOE Tri-Lab (ORNL, BNL, LANL) Research Effort to Provide
Accelerator-Produced Ac-225 for Radiotherapy
SO EUROPEAN JOURNAL OF NUCLEAR MEDICINE AND MOLECULAR IMAGING
LA English
DT Meeting Abstract
CT Annual Congress of the European-Association-of-Nuclear-Medicine
CY OCT 15-19, 2016
CL Barcelona, SPAIN
SP European Assoc Nucl Med
C1 [John, K. D.] Los Alamos Natl Lab, Los Alamos, NM USA.
NR 0
TC 0
Z9 0
U1 0
U2 0
PU SPRINGER
PI NEW YORK
PA 233 SPRING ST, NEW YORK, NY 10013 USA
SN 1619-7070
EI 1619-7089
J9 EUR J NUCL MED MOL I
JI Eur. J. Nucl. Med. Mol. Imaging
PD OCT
PY 2016
VL 43
SU 1
MA EP495
BP S419
EP S419
PG 1
WC Radiology, Nuclear Medicine & Medical Imaging
SC Radiology, Nuclear Medicine & Medical Imaging
GA EH5HE
UT WOS:000391802400493
ER
PT J
AU Armato, SG
Drukker, K
Li, F
Hadjiiski, L
Tourassi, GD
Engelmann, RM
Giger, ML
Redmond, G
Farahani, K
Kirby, JS
Clarke, LP
AF Armato, Samuel G., III
Drukker, Karen
Li, Feng
Hadjiiski, Lubomir
Tourassi, Georgia D.
Engelmann, Roger M.
Giger, Maryellen L.
Redmond, George
Farahani, Keyvan
Kirby, Justin S.
Clarke, Laurence P.
TI LUNGx Challenge for computerized lung nodule classification
SO JOURNAL OF MEDICAL IMAGING
LA English
DT Article
DE lung nodule; classification; computer-aided diagnosis; challenge;
computed tomography; image analysis
ID SOLITARY PULMONARY NODULES; CT SCANS; TOMOGRAPHY IMAGES; AIDED
DETECTION; SCREENING CT; SEGMENTATION; PERFORMANCE; PROBABILITY;
ALGORITHMS; EXTRACTION
AB The purpose of this work is to describe the LUNGx Challenge for the computerized classification of lung nodules on diagnostic computed tomography (CT) scans as benign or malignant and report the performance of participants' computerized methods along with that of six radiologists who participated in an observer study performing the same Challenge task on the same dataset. The Challenge provided sets of calibration and testing scans, established a performance assessment process, and created an infrastructure for case dissemination and result submission. Ten groups applied their own methods to 73 lung nodules (37 benign and 36 malignant) that were selected to achieve approximate size matching between the two cohorts. Area under the receiver operating characteristic curve (AUC) values for these methods ranged from 0.50 to 0.68; only three methods performed statistically better than random guessing. The radiologists' AUC values ranged from 0.70 to 0.85; three radiologists performed statistically better than the best-performing computer method. The LUNGx Challenge compared the performance of computerized methods in the task of differentiating benign from malignant lung nodules on CT scans, placed in the context of the performance of radiologists on the same task. The continued public availability of the Challenge cases will provide a valuable resource for the medical imaging research community. (C) 2016 Society of Photo-Optical Instrumentation Engineers (SPIE)
C1 [Armato, Samuel G., III; Drukker, Karen; Li, Feng; Engelmann, Roger M.; Giger, Maryellen L.] Univ Chicago, Dept Radiol, 5841 South Maryland Ave,MC 2026, Chicago, IL 60637 USA.
[Hadjiiski, Lubomir] Univ Michigan, Dept Radiol, 1500 East Med Ctr Dr, Ann Arbor, MI 48109 USA.
[Tourassi, Georgia D.] Biomed Sci & Engn Ctr, Hlth Data Sci Inst, Oak Ridge Natl Lab, POB 2008 MS6085, Oak Ridge, TN 37831 USA.
[Redmond, George; Farahani, Keyvan; Clarke, Laurence P.] NCI, Canc Imaging Program, Div Canc Treatment & Diag, 9609 Med Ctr Dr, Bethesda, MD 20892 USA.
[Kirby, Justin S.] Leidos Biomed Res Inc, Frederick Natl Lab Canc Res, Canc Imaging Program, 8560 Progress Dr, Frederick, MD 21702 USA.
RP Armato, SG (reprint author), Univ Chicago, Dept Radiol, 5841 South Maryland Ave,MC 2026, Chicago, IL 60637 USA.
EM s-armato@uchicago.edu
FU SPIE; AAPM; NCI; National Cancer Institute, National Institutes of
Health [HHSN261200800001E]; U.S. Department of Energy
[DE-AC05-00OR22725]
FX This paper is dedicated to the memory of Laurence P. Clarke, PhD, whose
vision helped shape not only the LUNGx Challenge but also, more
importantly, the broader imaging research landscape of open science,
consensus building, and collegiality that provides context for the
significance of grand challenges. He worked tirelessly to advance
research objectives by helping to surmount obstacles, building bridges
across institutions or governmental agencies, and selflessly advocating
on behalf of other investigators who shared his devotion to imaging
research. Dr. Clarke's career had a dramatic impact on the current state
of medical imaging research around the world. His leadership was
profound, his scientific contributions substantial, his intentions
sincere, his humor infectious, and his personality genuine; he will be
greatly missed by all his coauthors, colleagues, and friends. The
authors would like to express their appreciation to Angela Keyser and
Shayna Knazik from the AAPM and Diane Cline and Sandy Hoelterhoff from
the SPIE for their assistance in making this challenge a reality. The
LUNGx Challenge was supported by SPIE, AAPM, and NCI. The authors are
grateful to the groups that participated in the LUNGx Challenge,
including groups led by Yoganand Balagurunathan (H. Lee Moffitt Cancer
Center), Wookjin Choi (University of Maryland School of Medicine, now at
Memorial Sloan Kettering Cancer Center), Samuel Hawkins (University of
South Florida), Xiaojie Huang (GE Global Research), Lyndsey Pickup
(Mirada Medical, now at Optellum), Jiangdian Song (Northeastern
University, China), Yubing Tong (University of Pennsylvania), and Rafael
Wiemker (Philips Research Labs Hamburg). These participating groups
deserve recognition for their work to develop their lung nodule
classification methods and for their contributions to the success of the
Challenge. The authors would like to thank the radiologists who
participated in the observer study: Prachi Agarwal, MD, Aamer Chughtai,
MD, Jonathan Chung, MD, Heber MacMahon, MD, Steven Montner, MD, and
Smita Patel, MD. This project has been funded in whole or in part with
federal funds from the National Cancer Institute, National Institutes of
Health, under Contract No. HHSN261200800001E. The content of this
publication does not necessarily reflect the views or policies of the
Department of Health and Human Services, nor does mention of trade
names, commercial products, or organizations imply endorsement by the US
Government. This manuscript has been authored in part by UT-Battelle,
LLC under Contract No. DE-AC05-00OR22725 with the U.S. Department of
Energy. The US Government retains and the publisher, by accepting the
article for publication, acknowledges that the US Government retains a
nonexclusive, paid-up, irrevocable, worldwide license to publish or
reproduce the published form of this manuscript, or allow others to do
so, for US Government purposes. The Department of Energy will provide
public access to these results of federally sponsored research in
accordance with the DOE Public Access Plan
(http://energy.gov/downloads/doe-public-access-plan).
NR 39
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U1 3
U2 3
PU SPIE-SOC PHOTO-OPTICAL INSTRUMENTATION ENGINEERS
PI BELLINGHAM
PA 1000 20TH ST, PO BOX 10, BELLINGHAM, WA 98225 USA
SN 2329-4302
EI 2329-4310
J9 J MED IMAGING
JI J. Med. Imaging
PD OCT
PY 2016
VL 3
IS 4
AR UNSP 044506
DI 10.1117/1.JMI.3.4.044506
PG 9
WC Radiology, Nuclear Medicine & Medical Imaging
SC Radiology, Nuclear Medicine & Medical Imaging
GA EG5ZW
UT WOS:000391124500015
PM 28018939
ER
PT J
AU Tran, N
Giannakidis, A
Gullberg, GT
Seo, Y
AF Tran, Nicholas
Giannakidis, Archontis
Gullberg, Grant T.
Seo, Youngho
TI Quantitative analysis of hypertrophic myocardium using diffusion tensor
magnetic resonance imaging
SO JOURNAL OF MEDICAL IMAGING
LA English
DT Article
DE diffusion tensor magnetic resonance imaging; atlas; left ventricular
hypertrophy; spontaneous hypertensive rat
ID LEFT-VENTRICULAR HYPERTROPHY; SPONTANEOUSLY HYPERTENSIVE-RATS;
CARDIAC-HYPERTROPHY; LAMINAR STRUCTURE; HEART-FAILURE; FIBER;
CARDIOMYOPATHY; REGISTRATION; DYSFUNCTION; DEFORMATION
AB Systemic hypertension is a causative factor in left ventricular hypertrophy (LVH). This study is motivated by the potential to reverse or manage the dysfunction associated with structural remodeling of the myocardium in this pathology. Using diffusion tensor magnetic resonance imaging, we present an analysis of myocardial fiber and laminar sheet orientation in ex vivo hypertrophic (6 SHR) and normal (5 WKY) rat hearts using the covariance of the diffusion tensor. First, an atlas of normal cardiac microstructure was formed using the WKY b0 images. Then, the SHR and WKY b0 hearts were registered to the atlas. The acquired deformation fields were applied to the SHR and WKY heart tensor fields followed by the preservation of principal direction (PPD) reorientation strategy. A mean tensor field was then formed from the registered WKY tensor images. Calculating the covariance of the registered tensor images about this mean for each heart, the hypertrophic myocardium exhibited significantly increased myocardial fiber derangement (p = 0.017) with a mean dispersion of 38.7 deg, and an increased dispersion of the laminar sheet normal (p = 0.030) of 54.8 deg compared with 34.8 deg and 51.8 deg, respectively, in the normal hearts. Results demonstrate significantly altered myocardial fiber and laminar sheet structure in rats with hypertensive LVH. (C) 2016 Society of Photo-Optical Instrumentation Engineers (SPIE)
C1 [Tran, Nicholas; Gullberg, Grant T.; Seo, Youngho] Univ Calif San Francisco, Dept Radiol & Biomed Imaging, Phys Res Lab, 185 Berry St,Ste 350, San Francisco, CA 94143 USA.
[Giannakidis, Archontis] Royal Brompton Hosp, Cardiovasc Biomed Res Unit, Sydney St, London SW3 6NP, England.
[Giannakidis, Archontis] Imperial Coll London, Nat Heart & Lung Inst, Sydney St, London SW3 6NP, England.
[Giannakidis, Archontis; Gullberg, Grant T.; Seo, Youngho] Struct Biol & Imaging Dept, Lawrence Berkeley Natl Lab, 1 Cyclotron Rd, Berkeley, CA USA.
[Gullberg, Grant T.; Seo, Youngho] Univ Calif San Francisco, Joint Grad Grp Bioengn, 1700 4th St, San Francisco, CA 94143 USA.
[Seo, Youngho] Univ Calif San Francisco, Dept Radiat Oncol, 1600 Div St, San Francisco, CA 94143 USA.
RP Gullberg, GT (reprint author), Univ Calif San Francisco, Dept Radiol & Biomed Imaging, Phys Res Lab, 185 Berry St,Ste 350, San Francisco, CA 94143 USA.; Gullberg, GT (reprint author), Struct Biol & Imaging Dept, Lawrence Berkeley Natl Lab, 1 Cyclotron Rd, Berkeley, CA USA.; Gullberg, GT (reprint author), Univ Calif San Francisco, Joint Grad Grp Bioengn, 1700 4th St, San Francisco, CA 94143 USA.
EM gtgullberg@lbl.gov
FU National Heart, Lung, and Blood Institute [R01EB07219]; Office of
Science, Office of Biological and Environmental Research, Medical
Sciences Division of the US Department of Energy [DE-AC02-05CH11231]
FX The authors would like to thank Kathleen Brennan (LBNL) for harvesting
the samples, and Osama Abdullah and Edward Hsu (University of Utah, Salt
Lake City) for the diffusion tensor data collection. Additionally,
Michael Miller and Hangyi Jiang at Johns Hopkins University provided
valuable insight into the DiffeoMap software package. The authors would
also like to thank Damien Rohmer (Ecole Superieure de Chimie Physique
Eletronique de Lyon) for assisting with the tensor analysis. This work
was supported by the National Heart, Lung, and Blood Institute under
Grant R01EB07219, and by the Director, Office of Science, Office of
Biological and Environmental Research, Medical Sciences Division of the
US Department of Energy under Contract DE-AC02-05CH11231.
NR 50
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U1 1
U2 1
PU SPIE-SOC PHOTO-OPTICAL INSTRUMENTATION ENGINEERS
PI BELLINGHAM
PA 1000 20TH ST, PO BOX 10, BELLINGHAM, WA 98225 USA
SN 2329-4302
EI 2329-4310
J9 J MED IMAGING
JI J. Med. Imaging
PD OCT
PY 2016
VL 3
IS 4
AR 046001
DI 10.1117/1.JMI.3.4.046001
PG 10
WC Radiology, Nuclear Medicine & Medical Imaging
SC Radiology, Nuclear Medicine & Medical Imaging
GA EG5ZW
UT WOS:000391124500018
PM 27872872
ER
PT J
AU Qu, WC
Robert, CAM
Erb, M
Hibbard, BE
Paven, M
Gleede, T
Riehl, B
Kersting, L
Cankaya, AS
Kunert, AT
Xu, Y
Schueller, MJ
Shea, C
Alexoff, D
Lee, SJ
Fowler, JS
Ferrieri, RA
AF Qu, Wenchao
Robert, Christelle A. M.
Erb, Matthias
Hibbard, Bruce E.
Paven, Maxim
Gleede, Tassilo
Riehl, Barbara
Kersting, Lena
Cankaya, Aylin S.
Kunert, Anna T.
Xu, Youwen
Schueller, Michael J.
Shea, Colleen
Alexoff, David
Lee, So Jeong
Fowler, Joanna S.
Ferrieri, Richard A.
TI Dynamic Precision Phenotyping Reveals Mechanism of Crop Tolerance to
Root Herbivory
SO PLANT PHYSIOLOGY
LA English
DT Article
ID WESTERN CORN-ROOTWORM; AUXIN BIOSYNTHESIS; RAPID CHANGES;
ARABIDOPSIS-THALIANA; CARBON TRANSPORT; MICROPET R4; ACID; PLANTS;
TRYPTOPHAN; DAMAGE
AB The western corn rootworm (WCR; Diabrotica virgifera virgifera LeConte) is a major pest of maize (Zea mays) that is well adapted to most crop management strategies. Breeding for tolerance is a promising alternative to combat WCR but is currently constrained by a lack of physiological understanding and phenotyping tools. We developed dynamic precision phenotyping approaches using C-11 with positron emission tomography, root autoradiography, and radiometabolite flux analysis to understand maize tolerance to WCR. Our results reveal that WCR attack induces specific patterns of lateral root growth that are associated with a shift in auxin biosynthesis from indole-3-pyruvic acid to indole-3-acetonitrile. WCR attack also increases transport of newly synthesized amino acids to the roots, including the accumulation of Gln. Finally, the regrowth zones of WCR-attacked roots show an increase in Gln turnover, which strongly correlates with the induction of indole-3-acetonitrile-dependent auxin biosynthesis. In summary, our findings identify local changes in the auxin biosynthesis flux network as a promising marker for induced WCR tolerance.
C1 [Qu, Wenchao; Xu, Youwen; Schueller, Michael J.; Shea, Colleen; Alexoff, David; Lee, So Jeong; Fowler, Joanna S.; Ferrieri, Richard A.] Brookhaven Natl Lab, Dept Biol, Upton, NY 11973 USA.
[Robert, Christelle A. M.; Erb, Matthias] Univ Bern, Inst Plant Sci, Biot Interact, CH-3013 Bern, Switzerland.
[Hibbard, Bruce E.] Univ Missouri, USDA ARS, Plant Genet Res Unit, Columbia, MO 65211 USA.
[Paven, Maxim; Gleede, Tassilo; Riehl, Barbara; Kersting, Lena; Cankaya, Aylin S.; Kunert, Anna T.] Johannes Gutenberg Univ Mainz, Inst Kernchem, D-55128 Mainz, Germany.
[Qu, Wenchao] Cornell Univ, Weill Cornell Med, New York, NY 10065 USA.
[Paven, Maxim] Max Planck Inst Polymer Res, Ackermannweg 10, D-55128 Mainz, Germany.
[Kunert, Anna T.] Max Planck Inst Chem, Hahn Meitner Weg 1, D-55128 Mainz, Germany.
[Ferrieri, Richard A.] Univ Missouri, Dept Chem, MURR, 1513 Res Pk Dr, Columbia, MO 65211 USA.
[Lee, So Jeong] Univ Michigan, Dept Radiol, Med Ctr Dr, 1500 E Med Ctr Dr, Ann Arbor, MI 48109 USA.
RP Ferrieri, RA (reprint author), Brookhaven Natl Lab, Dept Biol, Upton, NY 11973 USA.; Ferrieri, RA (reprint author), Univ Missouri, Dept Chem, MURR, 1513 Res Pk Dr, Columbia, MO 65211 USA.
EM ferrierir@missouri.edu
RI MPIP, AK Butt/B-8805-2009
FU United States Department of Energy, Office of Biological and
Environmental Research [DE-AC02-98CH10886]; German Academic Exchange
Service (Deutscher Akademischer Austauschdienst, DAAD) Bonn; Marie Curie
Intra-European Fellowship program; Swiss National Foundation Fellowship
program; United States Government
FX This article has been authored by Brookhaven Science Associates, LLC,
under contract number DE-AC02-98CH10886 with the United States
Department of Energy, Office of Biological and Environmental Research.
Additional support was provided by the German Academic Exchange Service
(Deutscher Akademischer Austauschdienst, DAAD) Bonn, the Marie Curie
Intra-European Fellowship program, and the Swiss National Foundation
Fellowship program. The United States Government retains and the
publisher, by accepting the article for publication, acknowledges that
the United States Government retains a nonexclusive, paid-up,
irrevocable, world-wide license to publish or reproduce the published
form of this manuscript, or allow others to do so, for United States
Government purposes.
NR 54
TC 1
Z9 1
U1 11
U2 11
PU AMER SOC PLANT BIOLOGISTS
PI ROCKVILLE
PA 15501 MONONA DRIVE, ROCKVILLE, MD 20855 USA
SN 0032-0889
EI 1532-2548
J9 PLANT PHYSIOL
JI Plant Physiol.
PD OCT
PY 2016
VL 172
IS 2
BP 776
EP 788
DI 10.1104/pp.16.00735
PG 13
WC Plant Sciences
SC Plant Sciences
GA EG6II
UT WOS:000391147700013
PM 27406166
ER
PT J
AU Petri, A
AF Petri, A.
TI Mocking the weak lensing universe: The LensTools Python computing
package
SO ASTRONOMY AND COMPUTING
LA English
DT Article
DE Weak Gravitational Lensing; Simulations
ID SIMULATION CODE; POWER SPECTRUM; STATISTICS; PROBE; MCMC
AB We present a newly developed software package which implements a wide range of routines frequently used in Weak Gravitational Lensing (WL). With the continuously increasing size of the WL scientific community we feel that easy to use Application Program Interfaces (APIs) for common calculations are a necessity to ensure efficiency and coordination across different worldng groups. Coupled with existing open source codes, such as CAMB (Lewis et al., 2000) and Gadget2 (Springel, 2005), LensTools brings together a cosmic shear simulation pipeline which, complemented with a variety of WL feature measurement tools and parameter sampling routines, provides easy access to the numerics for theoretical studies of WL as well as for experiment forecasts. Being implemented in PYTHON (Rossum, 1995), LensTools takes full advantage of a range of state-of-the art techniques developed by the large and growing open-source software community (Jones et al., 2001; McKinney, 2010; Astrophy Collaboration, 2013; Pedregosa et al., 2011; Foreman-Mackey et al., 2013). We made the LensTools code available on the Python Package Index and published its documentation on http://lenstools.readthedocs.io. (C) 2016 Elsevier B.V. All rights reserved.
C1 [Petri, A.] Columbia Univ, Dept Phys, New York, NY 10027 USA.
[Petri, A.] Brookhaven Natl Lab, Dept Phys, Upton, NY 11973 USA.
RP Petri, A (reprint author), Columbia Univ, Dept Phys, New York, NY 10027 USA.
EM apetri@phys.columbia.edu
FU State of New York; U.S. Department of Energy [DE-AC02-98CH10886,
DESC0012704]; NSF [AST-1210877]; Research Opportunities and Approaches
to Data Science (ROADS) program at the Institute for Data Sciences and
Engineering at Columbia University; [ACI-1053575]
FX We thank Zoltan Haiman, Jia Liu, Jose M. Zorrilla and Morgan May for
invaluable support and useful discussions. The simulations in this work
were performed at the NSF Extreme Science and Engineering Discovery
Environment (XSEDE), supported by Grant Number ACI-1053575, at the Yeti
computing cluster at Columbia University, and at the New York Center for
Computational Sciences, a cooperative effort between Brookhaven National
Laboratory and Stony Brook University, supported in part by the State of
New York. This work was supported in part by the U.S. Department of
Energy under Contract Nos. DE-AC02-98CH10886 and DESC0012704, and by the
NSF Grant No. AST-1210877 (to Z.H.) and by the Research Opportunities
and Approaches to Data Science (ROADS) program at the Institute for Data
Sciences and Engineering at Columbia University.
NR 37
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Z9 3
U1 0
U2 0
PU ELSEVIER SCIENCE BV
PI AMSTERDAM
PA PO BOX 211, 1000 AE AMSTERDAM, NETHERLANDS
SN 2213-1337
EI 2213-1345
J9 ASTRON COMPUT
JI Astron. Comput.
PD OCT
PY 2016
VL 17
BP 73
EP 79
DI 10.1016/j.ascom.2016.06.001
PG 7
WC Astronomy & Astrophysics; Computer Science, Interdisciplinary
Applications
SC Astronomy & Astrophysics; Computer Science
GA EF9CD
UT WOS:000390627400002
ER
PT J
AU Nogales, E
Louder, RK
He, Y
AF Nogales, Eva
Louder, Robert K.
He, Yuan
TI Cryo-EM in the study of challenging systems: the human transcription
pre-initiation complex
SO CURRENT OPINION IN STRUCTURAL BIOLOGY
LA English
DT Article
ID RNA-POLYMERASE-II; TILT RECONSTRUCTION METHOD; AB-INITIO RECONSTRUCTION;
ELECTRON-MICROSCOPY; CORE PROMOTER; VISUALIZATION; RESOLUTION;
PARTICLES; CLASSIFICATION; SOFTWARE
AB Single particle cryo-Electron Microscopy (cryo-EM) is a technique that allows the structural characterization of macromolecules without the need for crystallization. For certain type of samples that are ideally suited for cryo-EM studies it has been possible to reach high-resolution structures following relatively standard procedures. Other biological systems remain highly challenging, even for cryo-EM. Challenges may involve the scarcity of the sample, poor stability of the complexes, and most often, the intrinsic flexibility of biological molecules. Among these challenging samples are large eukaryotic transcription complexes, which suffer from all such shortcomings. Here we report how we have recently tried to overcome those challenges in order to improve our structural understanding of the human transcription pre-initiation complex assembly and the transcription initiation process. Parallel efforts have also been carried out for budding yeast transcription initiation complexes, allowing comparisons that establish both the overall conservation and the specific structural differences between the two systems.
C1 [Nogales, Eva] Univ Calif Berkeley, Mol & Cell Biol Dept, Berkeley, CA 94720 USA.
[Nogales, Eva] Univ Calif Berkeley, Inst QB3, Berkeley, CA 94720 USA.
[Nogales, Eva] Univ Calif Berkeley, Howard Hughes Med Inst, Berkeley, CA 94720 USA.
[Nogales, Eva] Lawrence Berkeley Natl Lab, Mol Biophys & Integrat Bioimaging Div, Berkeley, CA 94720 USA.
[Louder, Robert K.] Univ Calif Berkeley, Biophys Grad Grp, Berkeley, CA USA.
[He, Yuan] Northwestern Univ, Dept Mol Biosci, Evanston, IL 60208 USA.
RP Nogales, E (reprint author), Univ Calif Berkeley, Mol & Cell Biol Dept, Berkeley, CA 94720 USA.; Nogales, E (reprint author), Univ Calif Berkeley, Inst QB3, Berkeley, CA 94720 USA.; Nogales, E (reprint author), Univ Calif Berkeley, Howard Hughes Med Inst, Berkeley, CA 94720 USA.; Nogales, E (reprint author), Lawrence Berkeley Natl Lab, Mol Biophys & Integrat Bioimaging Div, Berkeley, CA 94720 USA.
EM enogales@lbl.gov
FU NIGMS [GM63072]
FX This work was funded by NIGMS (GM63072 to EN). EN is a Howard Hughes
Medical Institute Investigator.
NR 37
TC 0
Z9 0
U1 10
U2 10
PU CURRENT BIOLOGY LTD
PI LONDON
PA 84 THEOBALDS RD, LONDON WC1X 8RR, ENGLAND
SN 0959-440X
EI 1879-033X
J9 CURR OPIN STRUC BIOL
JI Curr. Opin. Struct. Biol.
PD OCT
PY 2016
VL 40
BP 120
EP 127
DI 10.1016/j.sbi.2016.09.009
PG 8
WC Biochemistry & Molecular Biology; Cell Biology
SC Biochemistry & Molecular Biology; Cell Biology
GA EG0TI
UT WOS:000390744700017
PM 27689812
ER
PT J
AU Miller, ML
AF Miller, Mark L.
TI A Certified Health Physicist's Reflections on a 40-Year Career in
Radiation Protection
SO DOSE-RESPONSE
LA English
DT Article
DE LNT model; radiation hormesis; adaptive response; low-dose radiation
AB This is a reflection from a certified health physicist regarding his becoming aware, during his 40-year career, that the linear no-threshold (LNT) model and the associated As Low As Reasonably Achievable concept have no scientific basis and make no positive contribution to radiation safety. They should be replaced by an alternative, scientifically based model that includes a threshold, below which there is no harm, and recognition of hormesis and the adaptive response, which reflect the benefits of low-dose and low-dose-rate radiation exposure. Continued use of the unscientific LNT model is not conservative, as most regulators complacently claim but actually harmful. Examples of these harmful impacts in the areas of nuclear power, nuclear medicine, and environmental management are included.
C1 [Miller, Mark L.] Sandia Natl Labs, 620 La Jolla Pl NE, Albuquerque, NM 87123 USA.
RP Miller, ML (reprint author), Sandia Natl Labs, 620 La Jolla Pl NE, Albuquerque, NM 87123 USA.
EM marklmiller20@gmail.com
NR 10
TC 0
Z9 0
U1 4
U2 4
PU SAGE PUBLICATIONS INC
PI THOUSAND OAKS
PA 2455 TELLER RD, THOUSAND OAKS, CA 91320 USA
SN 1559-3258
J9 DOSE-RESPONSE
JI Dose-Response
PD OCT-DEC
PY 2016
VL 14
IS 4
DI 10.1177/1559325816673492
PG 3
WC Pharmacology & Pharmacy; Radiology, Nuclear Medicine & Medical Imaging;
Toxicology
SC Pharmacology & Pharmacy; Radiology, Nuclear Medicine & Medical Imaging;
Toxicology
GA EG3LI
UT WOS:000390944900003
ER
PT J
AU Van Weverberg, K
Boutle, IA
Morcrette, CJ
Newsom, RK
AF Van Weverberg, Kwinten
Boutle, Ian A.
Morcrette, Cyril J.
Newsom, Rob K.
TI Towards retrieving critical relative humidity from ground-based
remote-sensing observations
SO QUARTERLY JOURNAL OF THE ROYAL METEOROLOGICAL SOCIETY
LA English
DT Article
DE RHcrit; subgrid variability; parametrization; clouds; ARM; unified model
ID CONVECTIVE BOUNDARY-LAYER; WEATHER PREDICTION MODEL; TURBULENCE
CLOSURE-MODEL; ROTATIONAL RAMAN LIDAR; OFFICE UNIFIED MODEL; LARGE-SCALE
MODELS; VALLEY COLD POOLS; SCHEME DESCRIPTION; 4TH-ORDER MOMENTS;
WATER-VAPOR
AB Nearly all large-scale cloud parametrizations require the specification of the critical relative humidity (RHcrit). This is the grid-box mean relative humidity at which the subgrid fluctuations in temperature and water vapour are assumed to become so large that part of a subsaturated grid box becomes saturated and cloud starts to form. Until recently, the lack of high-resolution observations of temperature and moisture variability has hindered achievement of a reasonable estimate of RHcrit. However, the advent of ground-based Raman lidar now allows the acquisition of long records of temperature and moisture with subminute sample rates.
Lidar observations are inherently noisy and any analysis of higher-order moments will be dependent on the ability to quantify and remove this noise. We present an exploratory study aimed at understanding whether current noise levels of lidar-retrieved temperature and water vapour are sufficiently low to obtain a reasonable estimate of RHcrit. We show that vertical profiles of RHcrit can be derived with an uncertainty of a few per cent. RHcrit tends to be smallest near the boundary-layer top and seems to be insensitive to the horizontal grid spacing at the scales investigated here (30-120 km). However, larger sensitivity was found to the vertical grid spacing. RHcrit is observed to decrease by 10% as the vertical grid spacing quadruples.
By way of example, the lidar-retrieved RHcrit profiles were used to evaluate a parametrization that estimates RHcrit from variances diagnosed from the boundary-layer parametrization. It is shown that this parametrization overestimates RHcrit by up to 10%, but captures the diurnal variability of RHcrit well, with lower values of RHcrit near the boundary-layer top.
While we show that the uncertainties associated with the retrievals are large, lidar observations seem promising to diagnose and evaluate a very important parameter to predict cloud fraction in climate and numerical weather prediction models.
C1 [Van Weverberg, Kwinten; Boutle, Ian A.; Morcrette, Cyril J.] Met Off, Atmospher Proc & Parametrizat, Exeter, Devon, England.
[Newsom, Rob K.] Pacific Northwest Natl Lab, Atmospher Measurement & Data Sci, Richland, WA USA.
RP Van Weverberg, K (reprint author), Met Off, FitzRoy Rd, Exeter EX1 3PB, Devon, England.
EM kwinten.vanweverberg@metoffice.gov.uk
OI Boutle, Ian/0000-0002-1485-4475
FU DOE Office of Science, Office of Biological and Environmental Research,
Environmental Science Division
FX The authors are grateful to Dave Turner, Andreas Behrendt, Volker
Wulfmeyer, Simon Vosper and Adrian Lock for stimulating discussions. The
data for this article were gratefully obtained from the US Department of
Energy ARM data archive (http://www.archive.arm.gov/armlogin/login.jsp),
sponsored by the DOE Office of Science, Office of Biological and
Environmental Research, Environmental Science Division. We thank the
three anonymous reviewers for their constructive comments.
NR 47
TC 1
Z9 1
U1 3
U2 3
PU WILEY-BLACKWELL
PI HOBOKEN
PA 111 RIVER ST, HOBOKEN 07030-5774, NJ USA
SN 0035-9009
EI 1477-870X
J9 Q J ROY METEOR SOC
JI Q. J. R. Meteorol. Soc.
PD OCT
PY 2016
VL 142
IS 700
BP 2867
EP 2881
DI 10.1002/qj.2874
PN PT A
PG 15
WC Meteorology & Atmospheric Sciences
SC Meteorology & Atmospheric Sciences
GA EF9LU
UT WOS:000390652500022
ER
PT J
AU Romero-Severson, E
Bulla, I
Gromov, D
Serea, OS
Spicknall, I
AF Romero-Severson, Ethan
Bulla, Ingo
Gromov, Dmitry
Serea, Oana-Silvia
Spicknall, Ian
TI DYNAMIC ALLOCATION OF LIMITED HIV PREVENTION FUNDS USING CONTROL
THEORETIC METHODS
SO SEXUALLY TRANSMITTED DISEASES
LA English
DT Meeting Abstract
CT Sexually Transmitted Diseases (STD) Prevention Conference
CY SEP 20-23, 2016
CL Atlanta, GA
C1 [Romero-Severson, Ethan] Los Alamos Natl Lab, Theoret Biol & Biophys, Los Alamos, NM USA.
[Bulla, Ingo] Ernst Moritz Arndt Univ Greifswald, Greifswald, Germany.
[Gromov, Dmitry] St Petersburg State Univ, St Petersburg 199034, Russia.
[Serea, Oana-Silvia] Univ Perpignan, Perpignan, France.
[Spicknall, Ian] Ctr Dis Control & Prevent, Div STD Prevent, Atlanta, GA USA.
EM eoromero@lanl.gov
NR 0
TC 0
Z9 0
U1 0
U2 0
PU LIPPINCOTT WILLIAMS & WILKINS
PI PHILADELPHIA
PA TWO COMMERCE SQ, 2001 MARKET ST, PHILADELPHIA, PA 19103 USA
SN 0148-5717
EI 1537-4521
J9 SEX TRANSM DIS
JI Sex. Transm. Dis.
PD OCT
PY 2016
VL 43
SU 2
MA 2B5
BP S133
EP S133
PG 1
WC Infectious Diseases
SC Infectious Diseases
GA EG0BO
UT WOS:000390695900033
ER
PT J
AU Trinh, T
Perez, F
Luu, M
AF Thuy Trinh
Perez, Freddy
Minh Luu
TI SYPHILIS TESTING ALGORITHMS USED IN LABORATORIES IN LATIN AMERICA AND
THE CARIBEAN
SO SEXUALLY TRANSMITTED DISEASES
LA English
DT Meeting Abstract
CT Sexually Transmitted Diseases (STD) Prevention Conference
CY SEP 20-23, 2016
CL Atlanta, GA
C1 [Thuy Trinh] ORISE, Atlanta, GA USA.
[Perez, Freddy] Pan Amer Hlth Org, HIV Hepatitis TB & STI Unit, Washington, DC USA.
[Minh Luu] Emory Univ, Rollins Sch Publ Hlth, Dept Behav Sci & Hlth Educ, Atlanta, GA 30322 USA.
EM vfa2@cdc.gov
NR 0
TC 0
Z9 0
U1 0
U2 0
PU LIPPINCOTT WILLIAMS & WILKINS
PI PHILADELPHIA
PA TWO COMMERCE SQ, 2001 MARKET ST, PHILADELPHIA, PA 19103 USA
SN 0148-5717
EI 1537-4521
J9 SEX TRANSM DIS
JI Sex. Transm. Dis.
PD OCT
PY 2016
VL 43
SU 2
MA WP 92
BP S180
EP S180
PG 1
WC Infectious Diseases
SC Infectious Diseases
GA EG0BO
UT WOS:000390695900200
ER
PT J
AU Petaja, T
O'Connor, EJ
Moisseev, D
Sinclair, VA
Manninen, AJ
Vaananen, R
von Lerber, A
Thorntoton, JA
Nicocoll, K
Petersen, W
Chandrasekar, V
Smith, JN
Winkler, PM
Kruger, O
Hakola, H
Timonen, H
Brus, D
Laurila, T
Asmi, E
Riekkola, ML
Mona, L
Massoli, P
Engelmann, R
Komppppula, M
Wang, J
Kuang, CG
Back, J
Virtanen, A
Levula, J
Ritsche, M
Hickmon, N
AF Petaja, Tuukka
O'Connor, Ewan J.
Moisseev, Dmitri
Sinclair, Victoctoctoria A.
Manninen, Antttti J.
Vaananen, Riikka
von Lerber, Annakaisa
Thorntoton, Joel A.
Nicocoll, Keri
Petersen, Walt
Chandrasekar, V.
Smith, James N.
Winkler, Paul M.
Krueger, Olaf
Hakola, Hannele
Timonen, Hilkka
Brus, David
Laurila, Tuomas
Asmi, Eija
Riekkola, Marja-Liisa
Mona, Lucia
Massoli, Paola
Engelmann, Ronny
Komppppula, Mika
Wang, Jian
Kuang, Chongai
Baeck, Jaana
Virtanen, Annele
Levula, Janne
Ritsche, Michael
Hickmon, Nicki
TI BAECC A FIELD CAMPAIGN TO ELUCIDATE THE IMPACT OF BIOGENIC AEROSOLS ON
CLOUDS AND CLIMATE
SO BULLETIN OF THE AMERICAN METEOROLOGICAL SOCIETY
LA English
DT Article
ID NUCLEATION MODE PARTICLES; SECONDARY ORGANIC AEROSOL; GROUND-BASED
OBSERVATIONS; BOREAL FOREST SITE; SULFURIC-ACID; SCOTS PINE; ATMOSPHERIC
NUCLEATION; DOPPLER LIDAR; MASS-SPECTROMETER; CHERNOBYL FALLOUT
C1 [Petaja, Tuukka; Moisseev, Dmitri; Sinclair, Victoctoctoria A.; Manninen, Antttti J.; Vaananen, Riikka; Chandrasekar, V.; Krueger, Olaf; Levula, Janne] Univ Helsinki, Dept Phys, Gustaf Hallstromin Katu 2, Helsinki 00014, Finland.
[O'Connor, Ewan J.; Moisseev, Dmitri; von Lerber, Annakaisa; Chandrasekar, V.; Hakola, Hannele; Timonen, Hilkka; Brus, David; Laurila, Tuomas; Asmi, Eija] Finnish Meteorol Inst, Helsinki, Finland.
[O'Connor, Ewan J.; Nicocoll, Keri] Univ Reading, Dept Meteorol, Reading, Berks, England.
[Thorntoton, Joel A.] Univ Washington, Seattle, WA 98195 USA.
[Petersen, Walt] Natl Aeronaut & Space Adm, Goddard Space Flight Ctr, Wallops Flight Facil, Wallops Isl, VA USA.
[Chandrasekar, V.] Colorado State Univ, Ft Collins, CO 80523 USA.
[Smith, James N.] Natl Ctr Atmospher Res, POB 3000, Boulder, CO 80307 USA.
[Vaananen, Riikka; Smith, James N.] Univ Eastern Finland, Dept Appl Phys, Joensuu, Finland.
[Smith, James N.] Univ Calif Irvine, Irvine, CA USA.
[Winkler, Paul M.] Univ Vienna, Fac Phys, Vienna, Austria.
[Riekkola, Marja-Liisa] Univ Helsinki, Dept Analyt Chem, Helsinki, Finland.
[Mona, Lucia] Consiglio Nazl Ric Tito Scalo, Ist Metodol Anal Ambientale, Potenza, Italy.
[Massoli, Paola] Inst Atmospher Sci & Climate ISAC, Bologna, Italy.
[Massoli, Paola] Aerodyne Res Inc, Billerica, MA USA.
[Engelmann, Ronny] Leibniz Inst Tropospher Res, Leipzig, Germany.
[Komppppula, Mika] Finnish Meteorol Inst, Kuopio, Finland.
[Wang, Jian; Kuang, Chongai] Brookhaven Natl Lab, Upton, NY 11973 USA.
[Baeck, Jaana] Univ Helsinki, Dept Forest Sci, Helsinki, Finland.
[Levula, Janne] Stn Measuring Ecosyst Atmosphere Relat II, Hyytiala, Finland.
[Hickmon, Nicki] Argonne Natl Lab, Lemont, IL USA.
RP Petaja, T (reprint author), Univ Helsinki, Dept Phys, Gustaf Hallstromin Katu 2, Helsinki 00014, Finland.
EM tuukka.petaja@helsinki.fi
RI Virtanen, Annele/E-7699-2010; Petaja, Tuukka/A-8009-2008; Brus,
David/A-8296-2011; Smith, James/C-5614-2008; Wang, Jian/G-9344-2011;
OI Virtanen, Annele/0000-0002-2917-5344; Petaja,
Tuukka/0000-0002-1881-9044; Brus, David/0000-0002-8766-7873; Smith,
James/0000-0003-4677-8224; Manninen, Antti/0000-0003-3437-9189; Back,
Jaana/0000-0002-6107-667X; Sinclair, Victoria/0000-0002-2125-4726
FU Office of Science (BER), U.S. Department of Energy [DE-SC0011791,
DE-SC0014469]; European Commission; European Research Council via
NANO-DYNAMITE [616075]; Academy of Finland Centre of Excellence
[272041]; KONE foundation [46-6817]; Nordforsk via Cryosphere-Atmosphere
Interactions in a Changing Arctic Climate; CRAICC; TEKES in the
CLEEN/MMEA programme; Ministry of Transport and Communication through
ICOS-Finland; NASA Global Precipitation Measurement (GPM) mission ground
validation program; ARM; U.S. Department of Energy, Office of Science
and Technology [DE-AC02-06CH11357]
FX This work was partly supported by the Office of Science (BER), U.S.
Department of Energy via BAECC (Petaja), BAECC SNEX (Moisseev),
DE-SC0011791 (Thornton), DE-SC0014469 (Smith), and ASR (Chandrasekar);
European Commission via projects ACTRIS, ACTRIS-TNA, ACTRIS2, BACCHUS,
and PEGASOS and European Research Council via NANO-DYNAMITE (616075);
and Academy of Finland Centre of Excellence (Project 272041), KONE
foundation (Grant 46-6817), Nordforsk via Cryosphere-Atmosphere
Interactions in a Changing Arctic Climate, CRAICC, TEKES in the
CLEEN/MMEA programme, and the Ministry of Transport and Communication
through ICOS-Finland. The BAECC SNEX was also supported by NASA Global
Precipitation Measurement (GPM) mission ground validation program. The
deployment of AMF2 to Hyytiala was enabled and supported by ARM. Argonne
National Laboratory's work was supported by the U.S. Department of
Energy, Assistant Secretary for Environmental Management, Office of
Science and Technology, under Contract DE-AC02-06CH11357. The authors
gratefully acknowledge the support of AMF2, SMEAR II, and the BAECC
community for their support in initiating the BAECC campaign, its
implementation, operation, and data analysis.
NR 105
TC 1
Z9 1
U1 5
U2 5
PU AMER METEOROLOGICAL SOC
PI BOSTON
PA 45 BEACON ST, BOSTON, MA 02108-3693 USA
SN 0003-0007
EI 1520-0477
J9 B AM METEOROL SOC
JI Bull. Amer. Meteorol. Soc.
PD OCT
PY 2016
VL 97
IS 10
BP 1909
EP 1928
DI 10.1175/BAMS-D-14-00199.1
PG 20
WC Meteorology & Atmospheric Sciences
SC Meteorology & Atmospheric Sciences
GA ED9QR
UT WOS:000389208100011
ER
PT J
AU Patrignani, C
Agashe, K
Aielli, G
Amsler, C
Antonelli, M
Asner, DM
Baer, H
Banerjee, S
Barnett, RM
Basaglia, T
Bauer, CW
Beatty, JJ
Belousov, VI
Beringer, J
Bethke, S
Bichsel, H
Biebel, O
Blucher, E
Brooijmans, G
Buchmueller, O
Burkert, V
Bychkov, MA
Cahn, RN
Carena, M
Ceccucci, A
Cerri, A
Chakraborty, D
Chen, MC
Chivukula, RS
Copic, K
Cowan, G
Dahl, O
D'Ambrosio, G
Damour, T
de Florian, D
de Gouvea, A
DeGrand, T
de Jong, P
Dissertori, G
Dobrescu, BA
D'Onofrio, M
Doser, M
Drees, M
Dreiner, HK
Dwyer, DA
Eerola, P
Eidelman, S
Ellis, J
Erler, J
Ezhela, VV
Fetscher, W
Fields, BD
Foster, B
Freitas, A
Gallagher, H
Garren, L
Gerber, HJ
Gerbier, G
Gershon, T
Gherghetta, T
Godizov, AA
Goodman, M
Grab, C
Gritsan, AV
Grojean, C
Groom, DE
Grunewald, M
Gurtu, A
Gutsche, T
Haber, HE
Hagiwara, K
Hanhart, C
Hashimoto, S
Hayato, Y
Hayes, KG
Hebecker, A
Heltsley, B
Hernandez-Rey, JJ
Hikasa, K
Hisano, J
Hocker, A
Holder, J
Holtkamp, A
Huston, J
Hyodo, T
Irwin, K
Jackson, JD
Johnson, KF
Kado, M
Karliner, M
Katz, UF
Klein, SR
Klempt, E
Kowalewski, RV
Krauss, F
Kreps, M
Krusche, B
Kuyanov, YV
Kwon, Y
Lahav, O
Laiho, J
Langacker, P
Liddle, A
Ligeti, Z
Lin, CJ
Lippmann, C
Liss, TM
Littenberg, L
Lugovsky, KS
Lugovsky, SB
Lusiani, A
Makida, Y
Maltoni, F
Mannel, T
Manohar, AV
Marciano, WJ
Martin, AD
Masoni, A
Matthews, J
Meissner, UG
Milstead, D
Mitchell, RE
Molaro, P
Monig, K
Moortgat, F
Mortonson, MJ
Murayama, H
Nakamura, K
Narain, M
Nason, P
Navas, S
Neubert, M
Nevski, P
Nir, Y
Olive, KA
Griso, SP
Parsons, J
Peacock, JA
Pennington, M
Petcov, ST
Petrov, VA
Piepke, A
Pomarol, A
Quadt, A
Raby, S
Rademacker, J
Raffelt, G
Ratcliff, BN
Richardson, P
Ringwald, A
Roesler, S
Rolli, S
Romaniouk, A
Rosenberg, LJ
Rosner, JL
Rybka, G
Ryutin, RA
Sachrajda, CT
Sakai, Y
Salam, GP
Sarkar, S
Sauli, F
Schneider, O
Scholberg, K
Schwartz, AJ
Scott, D
Sharma, V
Sharpe, SR
Shutt, T
Silari, M
Sjostrand, T
Skands, P
Skwarnicki, T
Smith, JG
Smoot, GF
Spanier, S
Spieler, H
Spiering, C
Stahl, A
Stone, SL
Sumino, Y
Sumiyoshi, T
Syphers, MJ
Takahashi, F
Tanabashi, M
Terashi, K
Terning, J
Thorne, RS
Tiator, L
Titov, M
Tkachenko, NP
Tornqvist, NA
Tovey, D
Valencia, G
Van de Water, R
Varelas, N
Venanzoni, G
Vincter, MG
Vogel, P
Vogt, A
Wakely, SP
Walkowiak, W
Walter, CW
Wands, D
Ward, DR
Wascko, MO
Weiglein, G
Weinberg, DH
Weinberg, EJ
White, M
Wiencke, LR
Wiliocq, S
Wohl, CC
Wolfenstein, L
Womersley, J
Woody, CL
Workman, RL
Yao, WM
Zeller, GP
Zenin, OV
Zhu, RY
Zimmermann, F
Zyla, PA
Anderson, J
Harper, G
Lugovsky, VS
Schaffner, P
AF Patrignani, C.
Agashe, K.
Aielli, G.
Amsler, C.
Antonelli, M.
Asner, D. M.
Baer, H.
Banerjee, Sw.
Barnett, R. M.
Basaglia, T.
Bauer, C. W.
Beatty, J. J.
Belousov, V. I.
Beringer, J.
Bethke, S.
Bichsel, H.
Biebel, O.
Blucher, E.
Brooijmans, G.
Buchmueller, O.
Burkert, V.
Bychkov, M. A.
Cahn, R. N.
Carena, M.
Ceccucci, A.
Cerri, A.
Chakraborty, D.
Chen, M. -C.
Chivukula, R. S.
Copic, K.
Cowan, G.
Dahl, O.
D'Ambrosio, G.
Damour, T.
de Florian, D.
de Gouvea, A.
DeGrand, T.
de Jong, P.
Dissertori, G.
Dobrescu, B. A.
D'Onofrio, M.
Doser, M.
Drees, M.
Dreiner, H. K.
Dwyer, D. A.
Eerola, P.
Eidelman, S.
Ellis, J.
Erler, J.
Ezhela, V. V.
Fetscher, W.
Fields, B. D.
Foster, B.
Freitas, A.
Gallagher, H.
Garren, L.
Gerber, H. -J.
Gerbier, G.
Gershon, T.
Gherghetta, T.
Godizov, A. A.
Goodman, M.
Grab, C.
Gritsan, A. V.
Grojean, C.
Groom, D. E.
Gruenewald, M.
Gurtu, A.
Gutsche, T.
Haber, H. E.
Hagiwara, K.
Hanhart, C.
Hashimoto, S.
Hayato, Y.
Hayes, K. G.
Hebecker, A.
Heltsley, B.
Hernandez-Rey, J. J.
Hikasa, K.
Hisano, J.
Hoecker, A.
Holder, J.
Holtkamp, A.
Huston, J.
Hyodo, T.
Irwin, K.
Jackson, J. D.
Johnson, K. F.
Kado, M.
Karliner, M.
Katz, U. F.
Klein, S. R.
Klempt, E.
Kowalewski, R. V.
Krauss, F.
Kreps, M.
Krusche, B.
Kuyanov, Yu. V.
Kwon, Y.
Lahav, O.
Laiho, J.
Langacker, P.
Liddle, A.
Ligeti, Z.
Lin, C. -J.
Lippmann, C.
Liss, T. M.
Littenberg, L.
Lugovsky, K. S.
Lugovsky, S. B.
Lusiani, A.
Makida, Y.
Maltoni, F.
Mannel, T.
Manohar, A. V.
Marciano, W. J.
Martin, A. D.
Masoni, A.
Matthews, J.
Meissner, U. -G.
Milstead, D.
Mitchell, R. E.
Molaro, P.
Monig, K.
Moortgat, F.
Mortonson, M. J.
Murayama, H.
Nakamura, K.
Narain, M.
Nason, P.
Navas, S.
Neubert, M.
Nevski, P.
Nir, Y.
Olive, K. A.
Griso, S. Pagan
Parsons, J.
Peacock, J. A.
Pennington, M.
Petcov, S. T.
Petrov, V. A.
Piepke, A.
Pomarol, A.
Quadt, A.
Raby, S.
Rademacker, J.
Raffelt, G.
Ratcliff, B. N.
Richardson, P.
Ringwald, A.
Roesler, S.
Rolli, S.
Romaniouk, A.
Rosenberg, L. J.
Rosner, J. L.
Rybka, G.
Ryutin, R. A.
Sachrajda, C. T.
Sakai, Y.
Salam, G. P.
Sarkar, S.
Sauli, F.
Schneider, O.
Scholberg, K.
Schwartz, A. J.
Scott, D.
Sharma, V.
Sharpe, S. R.
Shutt, T.
Silari, M.
Sjostrand, T.
Skands, P.
Skwarnicki, T.
Smith, J. G.
Smoot, G. F.
Spanier, S.
Spieler, H.
Spiering, C.
Stahl, A.
Stone, S. L.
Sumino, Y.
Sumiyoshi, T.
Syphers, M. J.
Takahashi, F.
Tanabashi, M.
Terashi, K.
Terning, J.
Thorne, R. S.
Tiator, L.
Titov, M.
Tkachenko, N. P.
Tornqvist, N. A.
Tovey, D.
Valencia, G.
Van de Water, R.
Varelas, N.
Venanzoni, G.
Vincter, M. G.
Vogel, P.
Vogt, A.
Wakely, S. P.
Walkowiak, W.
Walter, C. W.
Wands, D.
Ward, D. R.
Wascko, M. O.
Weiglein, G.
Weinberg, D. H.
Weinberg, E. J.
White, M.
Wiencke, L. R.
Wiliocq, S.
Wohl, C. C.
Wolfenstein, L.
Womersley, J.
Woody, C. L.
Workman, R. L.
Yao, W. -M.
Zeller, G. P.
Zenin, O. V.
Zhu, R. -Y.
Zimmermann, F.
Zyla, P. A.
Anderson, J.
Harper, G.
Lugovsky, V. S.
Schaffner, P.
CA Particle Data Grp
TI REVIEW OF PARTICLE PHYSICS Particle Data Group
SO CHINESE PHYSICS C
LA English
DT Article
ID DEEP-INELASTIC-SCATTERING; SUPERSYMMETRIC STANDARD MODEL; PROTON-PROTON
COLLISIONS; TO-LEADING-ORDER; HIGGS-BOSON PRODUCTION; DOUBLE-BETA-DECAY;
GRAND UNIFIED THEORIES; CHIRAL PERTURBATION-THEORY; ELECTROWEAK
SYMMETRY-BREAKING; ANOMALOUS MAGNETIC-MOMENT
AB The Review summarizes much of particle physics and cosmology. Using data from previous editions, plus 3,062 new measurements from 721 papers, we list, evaluate, and average measured properties of gauge bosons and the recently discovered Higgs boson, leptons, quarks, mesons, and baryons. We summarize searches for hypothetical particles such as supersymmetric particles, heavy bosons, axions, dark photons, etc. All the particle properties and search limits are listed in Summary Tables. We also give numerous tables, figures, formulae, and reviews of topics such as Higgs Boson Physics, Supersymmetry, Grand Unified Theories, Neutrino Mixing, Dark Energy, Dark Matter, Cosmology, Particle Detectors, Colliders, Probability and Statistics. Among the 117 reviews are many that are new or heavily revised, including new reviews on Pentaquarks and Inflation. The complete Review is published online in a journal and on the website of the Particle Data Group (http://pdg.lbl.gov). The printed PDG Book contains the Summary Tables and all review articles but no longer includes the detailed tables from the Particle Listings. A Booklet with the Summary Tables and abbreviated versions of some of the review articles is also available.
C1 [Patrignani, C.] Univ Bologna, I-47921 Rimini, Italy.
[Patrignani, C.] INFN, Dip Sci Qualita Vita, I-47921 Rimini, Italy.
[Agashe, K.] Univ Maryland, Dept Phys, Coll Pk, College Pk, MD 20742 USA.
[Aielli, G.] Univ Roma Tor Vergata, Raimondo18, I-00173 Rome, Italy.
[Amsler, C.] Univ Bern, Albert Einstein Ctr Fundamental Phys, CH-3012 Bern, Switzerland.
[Amsler, C.] Austrian Acad Sci, Stefan Meyer Inst Subat Phys, Boltzmanngasse 3, A-1090 Vienna, Austria.
[Antonelli, M.; Venanzoni, G.] Lab Nazionali Frascati INFN, Via E. Fermi 40, I-00044 Frascati, Italy.
[Asner, D. M.] Pacif NW Natl Lab, 902 Battelle Blvd, Richland, WA 99352 USA.
[Baer, H.] Univ Oklahoma, Dept Phys & Astron, Norman, OK 73019 USA.
[Banerjee, Sw.] Univ Louisville, Louisville, KY 40292 USA.
[Barnett, R. M.; Bauer, C. W.; Beringer, J.; Cahn, R. N.; Ceccucci, A.; Copic, K.; Dahl, O.; Dwyer, D. A.; Groom, D. E.; Jackson, J. D.; Ligeti, Z.; Lin, C. -J.; Lugovsky, K. S.; Mortonson, M. J.; Murayama, H.; Griso, S. Pagan; Smoot, G. F.; Spieler, H.; White, M.; Wohl, C. C.; Yao, W. -M.; Zyla, P. A.; Anderson, J.; Harper, G.; Schaffner, P.] Lawrence Berkeley Natl Lab, Div Phys, 1 Cyclotron Rd, Berkeley, CA 94720 USA.
[Basaglia, T.; Ceccucci, A.; Cerri, A.; Doser, M.; Ellis, J.; Gurtu, A.; Hoecker, A.; Holtkamp, A.; Kado, M.; Moortgat, F.; Roesler, S.; Salam, G. P.; Sauli, F.; Silari, M.; Zimmermann, F.] CERN, European Org Nucl Res, CH-1211 Geneva 23, Switzerland.
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[Bethke, S.] Max Planck Inst Phys & Astrophys, D-80805 Munich, Germany.
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[Buchmueller, O.; Wascko, M. O.] Imperial Coll, Blackett Lab, High Energy Phys Grp, Prince Consort Rd, London SW7 2AZ, England.
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[Cowan, G.] Univ London, Dept Phys, Royal Holloway, Egham TW20 0EX, Surrey, England.
[D'Ambrosio, G.] INFN Sezione Napoli, Complesso Univ Monte St Angelo, Via Cintia, I-80126 Naples, Italy.
[Damour, T.] Inst Hautes Etud Sci, F-91440 Bures Sur Yvette, France.
[de Florian, D.] UNSAM, ICAS, 25 Mayo Francia, RA-1650 Buenos Aires, DF, Argentina.
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[de Jong, P.] Nikhef, POB 41882, NL-1009 DB Amsterdam, Netherlands.
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[D'Onofrio, M.] Univ Liverpool, Dept Phys, Oliver Lodge Lab, Oxford St, Liverpool L69 3BX, Merseyside, England.
[Drees, M.; Dreiner, H. K.] Univ Bonn, Physikal Inst, Nussallee 12, D-53115 Bonn, Germany.
[Eerola, P.] Univ Helsinki, Helsinki Inst Phys, POB 64, FIN-00014 Helsinki, Finland.
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[Ellis, J.] Kings Coll London, Dept Phys, London WC2R 2LS, England.
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[Foster, B.; Ringwald, A.; Weiglein, G.] Deutsch Elektronen Synchrotron DESY, Notkestrasse 85, D-22607 Hamburg, Germany.
[Foster, B.] Univ Oxford, Dept Phys, Denys Wilkinson Bldg, Oxford OX1 3RH, England.
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[Gerbier, G.; Titov, M.] CEA Saclay, DSM IRFU SPP, F-91191 Gif Sur Yvette, France.
[Gershon, T.; Kreps, M.] Univ Warwick, Dept Phys, Coventry CV4 7AL, W Midlands, England.
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[Hayato, Y.; Terashi, K.] Univ Tokyo, Dept Phys, Tokyo 1130033, Japan.
[Hayes, K. G.] Hillsdale Coll, Dept Phys, Hillsdale, MI 49242 USA.
[Hebecker, A.] Heidelberg Univ, Inst Theoret Phys, Philosophenweg 19, D-69120 Heidelberg, Germany.
[Heltsley, B.] Cornell Univ, Lab Elementary Particle Phys, Ithaca, NY 14853 USA.
[Hernandez-Rey, J. J.] Univ Valencia CSIC, IFIC Inst Fis Corpuscular, E-46071 Valencia, Spain.
[Hikasa, K.; Sumino, Y.; Takahashi, F.] Tohoku Univ, Dept Phys, Aoba Ku, Sendai, Miyagi 9808578, Japan.
[Hisano, J.; Tanabashi, M.] Nagoya Univ, Kobayashi Maskawa Inst, Chikusa Ku, Nagoya, Aichi 4640028, Japan.
[Holder, J.] Univ Delaware, Dept Phys & Astron, Newark, DE 19716 USA.
[Holder, J.] Univ Delaware, Bartol Res Inst, Newark, DE 19716 USA.
[Hyodo, T.] Kyoto Univ, Yukawa Inst Theoret Phys, Sakyo Ku, Kitashirakawa Oiwakecho, Kyoto 6068502, Japan.
[Irwin, K.] Stanford Univ, Dept Phys, Stanford, CA 94305 USA.
[Irwin, K.; Ratcliff, B. N.; Shutt, T.] SLAC Natl Accelerator Lab, 2575 Sand Hill Rd, Menlo Pk, CA 94025 USA.
[Johnson, K. F.] Los Alamos Natl Lab, Los Alamos, NM 87545 USA.
[Kado, M.] Univ Paris 11, F-91898 Orsay, France.
[Kado, M.] CNRS, IN2P3, LAL, F-91898 Orsay, France.
[Karliner, M.] Tel Aviv Univ, Dept Particle Phys, IL-69978 Tel Aviv, Israel.
[Katz, U. F.] Univ Erlangen Nurnberg, Erlangen Ctr Astroparticle Phys, Erwin Rommel Str 1, D-91058 Erlangen, Germany.
[Klein, S. R.] Lawrence Berkeley Natl Lab, Div Nucl Sci, 1 Cyclotron Rd, Berkeley, CA 94720 USA.
[Klempt, E.; Meissner, U. -G.] Univ Bonn, Helmholtz Inst Strahlen & Kernphysik, Nussallee 14-16, D-53115 Bonn, Germany.
[Kowalewski, R. V.] Univ Victoria, Victoria, BC V8W 3P6, Canada.
[Krauss, F.; Martin, A. D.; Richardson, P.] Univ Durham, Dept Phys, Inst Particle Phys Phenomenol, Durham DH1 3LE, England.
[Krusche, B.] Univ Basel, Inst Phys, CH-4056 Basel, Switzerland.
[Kwon, Y.] Yonsei Univ, Dept Phys, 134 Sinchon dong, Seoul 120749, South Korea.
[Lahav, O.; Thorne, R. S.] UCL, Dept Phys & Astron, Gower St, London WC1E 6BT, England.
[Laiho, J.; Skwarnicki, T.; Stone, S. L.] Syracuse Univ, Dept Phys, Syracuse, NY 13244 USA.
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[Lusiani, A.] INFN, I-56127 Pisa, Italy.
[Maltoni, F.] Catholic Univ Louvain, Ctr Cosmol, Particle Phys & Phenomenol CP3, B-1348 Louvain, Belgium.
[Mannel, T.; Walkowiak, W.] Univ Siegen, Dept Physik, Walter Flex Str 3, D-57068 Siegen, Germany.
[Manohar, A. V.; Sharma, V.] Univ Calif San Diego, Dept Phys, La Jolla, CA 92093 USA.
[Masoni, A.] Cittadella Univ Monserrato, INFN, Sez Cagliari, I-09042 Monserrato, Italy.
[Matthews, J.] Louisiana State Univ, Dept Phys & Astron, Baton Rouge, LA 70803 USA.
[Milstead, D.] AlbaNova Univ Ctr, Stockholm Univ, Fysikum, SE-10691 Stockholm, Sweden.
[Mitchell, R. E.] Indiana Univ, Dept Phys, 727 E 3rd St, Bloomington, IN 47405 USA.
[Molaro, P.] INAF OATS, Via GB Tiepolo 11, I-34143 Trieste, Italy.
[Monig, K.; Spiering, C.] DESY, D-15735 Zeuthen, Germany.
[Mortonson, M. J.] Univ Calif Berkeley, SSL, 7 Gauss Way, Berkeley, CA 94720 USA.
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[Murayama, H.; Smoot, G. F.; White, M.] Univ Calif Berkeley, Dept Phys, Berkeley, CA 94720 USA.
[Narain, M.] Brown Univ, Dept Phys, 182 Hope St, Providence, RI 02912 USA.
[Nason, P.] INFN, Sez Milano Bicocca, Piazza Scienza, I-20126 Milan, Italy.
[Navas, S.] Univ Granada, Dpto Fis Teor Cosmos & CAFPE, Granada 18071, Spain.
[Neubert, M.] Johannes Gutenberg Univ Mainz, Mainz Inst Theoret Phys, D-55099 Mainz, Germany.
[Neubert, M.] Johannes Gutenberg Univ Mainz, PRISMA Cluster Excellence, D-55099 Mainz, Germany.
[Nir, Y.] Weizmann Inst Sci, Dept Particle Phys & Astrophys, IL-7610001 Rehovot, Israel.
[Petcov, S. T.] Ist Nazl Fis Nucl, SISSA, Via Bonomea 265, I-34136 Trieste, Italy.
[Petcov, S. T.] Bulgarian Acad Sci, INRNE, Sofia 1784, Bulgaria.
[Piepke, A.] Univ Alabama, Dept Phys & Astron, 206 Gallalee Hall, Tuscaloosa, AL 35487 USA.
[Pomarol, A.] Univ Autonoma Barcelona, Dept Fis, Barcelona 08193, Spain.
[Quadt, A.] Univ Gottingen, II Physikal Inst, Friedrich Hund Platz 1, D-37077 Gottingen, Germany.
[Rademacker, J.] Univ Bristol, HH Wills Phys Lab, Tyndall Ave, Bristol BS8 1TL, Avon, England.
Max Planck Inst Physik Werner Heisenberg Inst, Fohringer Ring 6, D-80805 Munich, Germany.
[Rolli, S.] DOE, 1000 Independence Ave,SW,SC-25 Germantown Bldg, Washington, DC 20585 USA.
[Romaniouk, A.] Natl Res Nucl Univ, MEPhI, 31 Kashirskoye Shosse, Moscow 115409, Russia.
[Sachrajda, C. T.] Univ Southampton, Sch Phys & Astron, Southampton S017 1BJ, Hants, England.
[Salam, G. P.] UPMC Univ Paris 6, CNRS UMR 7589, LPTHE, 4 Pl Jussieu, Paris, France.
[Sarkar, S.] Univ Oxford, Rudolf Peierls Ctr Theoret Phys, 1 Keble Rd, Oxford OX1 3NP, England.
[Sarkar, S.] Niels Bohr Inst, Blegdamsvej 17, DK-2100 Copenhagen, Denmark.
[Schneider, O.] Ecole Polytech Fed Lausanne, CH-1015 Lausanne, Switzerland.
[Scholberg, K.; Walter, C. W.] Duke Univ, Dept Phys, Durham, NC 27708 USA.
[Schwartz, A. J.] Univ Cincinnati, Dept Phys, 400 Geology Phys Bldg, Cincinnati, OH 45221 USA.
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[Sjostrand, T.] Lund Univ, Dept Astron & Theoret Phys, S-22362 Lund, Sweden.
[Skands, P.; Valencia, G.] Monash Univ, Sch Phys, Melbourne, Vic 3800, Australia.
[Smoot, G. F.] Univ Paris 04, Univ Paris Diderot, CNRS, Paris Ctr Cosmol Phys,APC, F-75013 Paris, France.
[Spanier, S.] Univ Tennessee, Dept Phys & Astron, Knoxville, TN 37996 USA.
[Stahl, A.] Rhein Westfal TH Aachen, III Physikal Inst, Physikzentrum, D-52056 Aachen, Germany.
[Sumiyoshi, T.] Tokyo Metropolitan Univ, High Energy Phys Lab, Tokyo 1920397, Japan.
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[Tiator, L.] Johannes Gutenberg Univ Mainz, Inst Kernphysik, D-55099 Mainz, Germany.
[Tovey, D.] Univ Sheffield, Dept Phys & Astron, Sheffield S3 7RH, S Yorkshire, England.
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[Wands, D.] Univ Portsmouth, Inst Cosmol & Gravitat, Burnaby Rd, Portsmouth PO1 3FX, Hants, England.
[Ward, D. R.] Cavendish Lab, J J Thomson Ave, Cambridge CB3 0HE, England.
[Weinberg, D. H.] Ohio State Univ, CCAPP, 140 W 18th Ave, Columbus, OH 43210 USA.
[Weinberg, D. H.] Ohio State Univ, Dept Astron, 140 W 18th Ave, Columbus, OH 43210 USA.
[Wiencke, L. R.] Colorado Sch Mines, Dept Phys, Golden, CO 80401 USA.
[Wiliocq, S.] Univ Massachusetts, Dept Phys, 1126 Lederle Grad Res Tower, Amherst, MA 01003 USA.
[Wolfenstein, L.] Carnegie Mellon Univ, Dept Phys, Pittsburgh, PA 15213 USA.
[Womersley, J.] STFC Rutherford Appleton Lab, Didcot OX11 0QX, Oxon, England.
[Workman, R. L.] George Washington Univ, Dept Phys, Virginia Campus, Ashburn, VA 20147 USA.
[Zhu, R. -Y.] CALTECH, High Energy Phys, MC 256 48, Pasadena, CA 91125 USA.
RP Patrignani, C (reprint author), Univ Bologna, I-47921 Rimini, Italy.
RI Sarkar, Subir/G-5978-2011; White, Martin/I-3880-2015; Patrignani,
Claudia/C-5223-2009; Beatty, James/D-9310-2011; Navas,
Sergio/N-4649-2014
OI Sarkar, Subir/0000-0002-3542-858X; White, Martin/0000-0001-9912-5070;
Patrignani, Claudia/0000-0002-5882-1747; Beatty,
James/0000-0003-0481-4952; Navas, Sergio/0000-0003-1688-5758
FU Office of Science, Office of High Energy Physics of the U.S. Department
of Energy [DE-AC02-05CH11231]; European Laboratory for Particle Physics
(CERN); government of Japan (MEXT: Ministry of Education, Culture,
Sports, Science and Technology); government of United States (DOE) on
cooperative research and development; Institute of High Energy Physics,
Chinese Academy of Sciences; Italian National Institute of Nuclear
Physics (INFN)
FX The publication of the Review of Particle Physics is supported by the
Director, Office of Science, Office of High Energy Physics of the U.S.
Department of Energy under Contract No. DE-AC02-05CH11231; by the
European Laboratory for Particle Physics (CERN); by an implementing
arrangement between the governments of Japan (MEXT: Ministry of
Education, Culture, Sports, Science and Technology) and the United
States (DOE) on cooperative research and development; by the Institute
of High Energy Physics, Chinese Academy of Sciences; and by the Italian
National Institute of Nuclear Physics (INFN).
NR 8419
TC 96
Z9 98
U1 44
U2 44
PU CHINESE PHYSICAL SOC
PI BEIJING
PA P O BOX 603, BEIJING 100080, PEOPLES R CHINA
SN 1674-1137
J9 CHINESE PHYS C
JI Chin. Phys. C
PD OCT
PY 2016
VL 40
IS 10
AR 100001
DI 10.1088/1674-1137/40/10/100001
PG 1790
WC Physics, Nuclear; Physics, Particles & Fields
SC Physics
GA EB2XR
UT WOS:000387226400001
ER
PT J
AU Auerbach, DA
Buchanan, BP
Alexiades, AV
Anderson, EP
Encalada, AC
Larson, EI
McManamay, RA
Poe, GL
Walter, MT
Flecker, AS
AF Auerbach, Daniel A.
Buchanan, Brian P.
Alexiades, Alexander V.
Anderson, Elizabeth P.
Encalada, Andrea C.
Larson, Erin I.
McManamay, Ryan A.
Poe, Gregory L.
Walter, M. Todd
Flecker, Alexander S.
TI Towards catchment classification in data-scarce regions
SO ECOHYDROLOGY
LA English
DT Article
DE environmental classification; hydroclimate; flow regime; Colorado;
Ecuador
ID NATURAL FLOW REGIMES; HYDROLOGICAL CLASSIFICATION; BIODIVERSITY
CONSERVATION; FRAMEWORK; RIVERS; MAP
AB Assessing spatial variation in hydrologic processes can help to inform freshwater management and advance ecological understanding, yet many areas lack sufficient flow records on which to base classifications. Seeking to address this challenge, we apply concepts developed in data-rich settings to public, global data in order to demonstrate a broadly replicable approach to characterizing hydrologic variation. The proposed approach groups the basins associated with reaches in a river network according to key environmental drivers of hydrologic conditions. This initial study examines Colorado ( USA), where long-term streamflow records permit comparison with previously distinguished flow regime types, and Ecuador, where data limitations preclude such analysis. The flow regime types assigned to gages in Colorado corresponded reasonably well to the classes distinguished from environmental features. The divisions in Ecuador reflected major known biophysical gradients while also providing a higher resolution supplement to an existing depiction of freshwater ecoregions. Although freshwater policy and management decisions occur amidst uncertainty and imperfect knowledge, this classification framework offers a rigorous and transferrable means to distinguish catchments in data-scarce regions. The maps and attributes of the resulting ecohydrologic classes offer a departure point for additional study and data collection programmes such as the placement of stations in under-monitored classes, and the divisions may serve as a preliminary template with which to structure conservation efforts such as environmental flow assessments. Copyright (C) 2015 John Wiley & Sons, Ltd.
C1 [Auerbach, Daniel A.; Larson, Erin I.; Flecker, Alexander S.] Cornell Univ, Dept Ecol & Evolutionary Biol, Ithaca, NY 14850 USA.
[Buchanan, Brian P.; Walter, M. Todd] Cornell Univ, Dept Biol & Environm Engn, Ithaca, NY USA.
[Alexiades, Alexander V.] Cornell Univ, Dept Nat Resources, Fernow Hall, Ithaca, NY 14853 USA.
[Anderson, Elizabeth P.] Florida Int Univ, Sch Environm Arts & Soc, Miami, FL 33199 USA.
[Encalada, Andrea C.] Univ San Francisco Quito, Lab Ecol Acuat, Colegio Ciencias Biol & Ambientales, Quito, Ecuador.
[McManamay, Ryan A.] Oak Ridge Natl Lab, Div Environm Sci, POB 2008, Oak Ridge, TN 37831 USA.
[Poe, Gregory L.] Cornell Univ, Dyson Sch Appl Econ & Management, Ithaca, NY USA.
US EPA, Off Wetlands Oceans & Watersheds, Washington, DC 20460 USA.
Heritage Univ, Dept Environm Sci, Toppenish, WA, Australia.
RP Auerbach, DA (reprint author), Cornell Univ, Dept Ecol & Evolutionary Biol, Ithaca, NY 14850 USA.
EM da373@cornell.edu
OI Larson, Erin/0000-0002-7797-0529; Auerbach, Daniel/0000-0002-3655-5206;
Encalada, Andrea C./0000-0003-2497-6086
FU Atkinson Centre for a Sustainable Future at Cornell University;
Dimensions of Biodiversity EVOTRAC project [NSF 1045960, NSF 1046408,
NSF 1046991]; Nature Conservancy NatureNet fellowship
FX This research was stimulated by a workshop in Quito supported by the
Atkinson Centre for a Sustainable Future at Cornell University and the
Dimensions of Biodiversity EVOTRAC project (NSF 1045960, NSF 1046408,
and NSF 1046991). We thank all workshop participants for their
contributions to understanding Andean environmental flow needs. DA is
grateful for support from The Nature Conservancy NatureNet fellowship.
Heather Tallis and Spencer Meyer offered thoughtful suggestions that
greatly improved the manuscript. We thank Jacob Bien and Erika Mudrak
for valuable conversation regarding statistical options.
NR 40
TC 0
Z9 0
U1 4
U2 4
PU WILEY-BLACKWELL
PI HOBOKEN
PA 111 RIVER ST, HOBOKEN 07030-5774, NJ USA
SN 1936-0584
EI 1936-0592
J9 ECOHYDROLOGY
JI Ecohydrology
PD OCT
PY 2016
VL 9
IS 7
BP 1235
EP 1247
DI 10.1002/eco.1721
PG 13
WC Ecology; Environmental Sciences; Water Resources
SC Environmental Sciences & Ecology; Water Resources
GA EF0NF
UT WOS:000390021700008
ER
PT J
AU Bao, J
Xu, ZJ
Fang, YL
AF Bao, Jie
Xu, Zhijie
Fang, Yilin
TI A coupled thermal-hydromechanical simulation for carbon dioxide
sequestration
SO ENVIRONMENTAL GEOTECHNICS-JOURNAL
LA English
DT Article
DE numerical methods; waste containment and disposal system
ID FINITE-ELEMENT METHODS; DEEP SALINE AQUIFERS; GEOLOGICAL SEQUESTRATION;
GEOMECHANICAL RESPONSE; FAULT REACTIVATION; CO2 SEQUESTRATION;
FLUID-FLOW; INJECTION; CONSOLIDATION; DEFORMATION
AB Herein, the authors present a coupled thermal-hydro-mechanical model, as an improvement of the isotherm hydromechanical model in their previous work, for geological sequestration of carbon dioxide followed by stress, deformation, and shear-slip failure analyses. This fully coupled model considers the geomechanical response, fluid flow and thermal transport relevant to geological sequestration. Both analytical solutions and numerical approach by way of finite element model are introduced for solving the thermal-hydro-mechanical model. Analytical solutions for pressure, temperature, deformation and stress field were obtained for a simplified typical geological sequestration scenario by assuming a simplified temperature profile in an aquifer. The finite element model is more general and can be used for arbitrary geometry. It was built on an open-source finite element solver, Elmer, and was designed to simulate the entire period of carbon dioxide injection both stably and accurately - even for large time steps. The shear-slip failure analysis was implemented based on the numerical results from the finite element model. The analysis reveals the potential failure zone caused by the fluid injection and thermal effect. From the simulation results, the thermal effect is shown to reduce the potential failure zone, especially at the early time of the injection.
C1 [Bao, Jie] Pacific Northwest Natl Lab, Expt & Computat Engn Grp, Energy & Environm Directorate, Richland, WA 99352 USA.
[Xu, Zhijie] Pacific Northwest Natl Lab, Computat Math Grp, Fundamental & Computat Sci Directorate, Richland, WA USA.
[Fang, Yilin] Pacific Northwest Natl Lab, Hydrol Tech Grp, Energy & Environm Directorate, Richland, WA USA.
RP Bao, J (reprint author), Pacific Northwest Natl Lab, Expt & Computat Engn Grp, Energy & Environm Directorate, Richland, WA 99352 USA.
FU Pacific Northwest National Laboratory (PNNL) Carbon Sequestration
Initiative part of the Laboratory Directed Research and Development
Program; U.S. Department of Energy [DE-AC05-76RL01830]
FX This research was funded and conducted through the Pacific Northwest
National Laboratory (PNNL) Carbon Sequestration Initiative, which is
part of the Laboratory Directed Research and Development Program. PNNL
is operated by Battelle for the U.S. Department of Energy under Contract
DE-AC05-76RL01830.
NR 42
TC 1
Z9 1
U1 0
U2 0
PU ICE PUBLISHING
PI WESTMINISTER
PA INST CIVIL ENGINEERS, 1 GREAT GEORGE ST, WESTMINISTER SW 1P 3AA, ENGLAND
SN 2051-803X
J9 ENVIRON GEOTECH-J
JI Environ. Geotech.-J.
PD OCT
PY 2016
VL 3
IS 5
BP 312
EP 324
AR 14.00002
DI 10.1680/envgeo.14.00002
PG 13
WC Engineering, Geological
SC Engineering
GA EF3SJ
UT WOS:000390244400004
ER
PT J
AU Fowler, TK
Li, H
AF Fowler, T. Kenneth
Li, Hui
TI Spheromaks and how plasmas may explain the ultra high energy cosmic ray
mystery
SO JOURNAL OF PLASMA PHYSICS
LA English
DT Article
DE accretion disk; cosmic rays; spheromak
ID QUASI-STATIC MODEL; COLLIMATED JETS; DISCS
AB In recent papers, we show how accretion disks around massive black holes could act as dynamos producing magnetic jets similar to the jets that create spheromaks in the laboratory. In this paper, we discuss how these magnetic astrophysical jets might naturally produce runaway ion beams accelerated to 10(20) eV or more, finally ejected as ultra high energy cosmic rays (UHECRs) long regarded as one of the mysteries of astrophysics. The acceleration is mainly due to the drift cyclotron loss cone kinetic instability known from plasma research. Experiments and simulations are suggested to verify the acceleration process.
C1 [Fowler, T. Kenneth] Univ Calif Berkeley, Berkeley, CA 94720 USA.
[Li, Hui] Los Alamos Natl Lab, Los Alamos, NM 87545 USA.
RP Li, H (reprint author), Los Alamos Natl Lab, Los Alamos, NM 87545 USA.
EM hli@lanl.gov
NR 21
TC 0
Z9 0
U1 1
U2 1
PU CAMBRIDGE UNIV PRESS
PI NEW YORK
PA 32 AVENUE OF THE AMERICAS, NEW YORK, NY 10013-2473 USA
SN 0022-3778
EI 1469-7807
J9 J PLASMA PHYS
JI J. Plasma Phys.
PD OCT
PY 2016
VL 82
AR 595820503
DI 10.1017/S0022377816000866
PN 5
PG 9
WC Physics, Fluids & Plasmas
SC Physics
GA EF5PZ
UT WOS:000390383400005
ER
PT J
AU Vaivads, A
Retino, A
Soucek, J
Khotyaintsev, YV
Valentini, F
Escoubet, CP
Alexandrova, O
Andre, M
Bale, SD
Balikhin, M
Burgessl, D
Camporeale, E
Caprioli, D
Chen, CHK
Clacey, E
Cully, CM
De Keyser, J
Eastwood, JP
Fazakerley, AN
Eriksson, S
Goldstein, ML
Graham, DB
Haaland, S
Hoshino, M
Ji, H
Karimabadi, H
Kucharek, H
Lavraud, B
Marcucci, F
Matthaeus, WH
Moore, TE
Nakamura, R
Narita, Y
Nemecek, Z
Norgren, C
Opgenoorth, H
Palmroth, M
Perrone, D
Pinqon, JL
Rathsman, P
Rothkaeh, H
Sahraoui, F
Servidio, S
Sorriso-Valvo, L
Vainio, R
Voros, Z
Wimmer-Schweingruber, RF
AF Vaivads, A.
Retino, A.
Soucek, J.
Khotyaintsev, Yu. V.
Valentini, F.
Escoubet, C. P.
Alexandrova, O.
Andre, M.
Bale, S. D.
Balikhin, M.
Burgessl, D.
Camporeale, E.
Caprioli, D.
Chen, C. H. K.
Clacey, E.
Cully, C. M.
De Keyser, J.
Eastwood, J. P.
Fazakerley, A. N.
Eriksson, S.
Goldstein, M. L.
Graham, D. B.
Haaland, S.
Hoshino, M.
Ji, H.
Karimabadi, H.
Kucharek, H.
Lavraud, B.
Marcucci, F.
Matthaeus, W. H.
Moore, T. E.
Nakamura, R.
Narita, Y.
Nemecek, Z.
Norgren, C.
Opgenoorth, H.
Palmroth, M.
Perrone, D.
Pinqon, J. -L.
Rathsman, P.
Rothkaeh, H.
Sahraoui, F.
Servidio, S.
Sorriso-Valvo, L.
Vainio, R.
Voeroes, Z.
Wimmer-Schweingruber, R. F.
TI Turbulence Heating ObserveR - satellite mission proposal
SO JOURNAL OF PLASMA PHYSICS
LA English
DT Article
DE plasma heating; plasma properties; space plasma physics
ID SOLAR-WIND; PLASMA TURBULENCE; TEMPERATURE ANISOTROPY; VLASOV
SIMULATIONS; ELECTRON SCALES; ION; MAGNETOSHEATH; FLUCTUATIONS;
FORESHOCK
AB The Universe is permeated by hot, turbulent, magnetized plasmas. Turbulent plasma is a major constituent of active galactic nuclei, supernova remnants, the intergalactic and interstellar medium, the solar corona, the solar wind and the Earth's magnetosphere, just to mention a few examples. Energy dissipation of turbulent fluctuations plays a key role in plasma heating and energization, yet we still do not understand the underlying physical mechanisms involved. THOR is a mission designed to answer the questions of how turbulent plasma is heated and particles accelerated, how the dissipated energy is partitioned and how dissipation operates in different regimes of turbulence. THOR is a single-spacecraft mission with an orbit tuned to maximize data return from regions in near-Earth space - magnetosheath, shock, foreshock and pristine solar wind - featuring different kinds of turbulence. Here we summarize the THOR proposal submitted on 15 January 2015 to the 'Call for a Medium-size mission opportunity in ESAs Science Programme for a launch in 2025 (M4)'. THOR has been selected by European Space Agency (ESA) for the study phase.
C1 [Vaivads, A.; Khotyaintsev, Yu. V.; Andre, M.; Graham, D. B.; Norgren, C.; Opgenoorth, H.] Swedish Inst Space Phys, S-75121 Uppsala, Sweden.
[Retino, A.; Sahraoui, F.] Ecole Polytech, Lab Phys Plasmas, F-91128 Palaiseau, France.
[Soucek, J.] Acad Sci Czech Republic, Inst Atmospher Phys, CZ-14131 Prague, Czech Republic.
[Valentini, F.; Servidio, S.] Univ Calabria, Dipartimento Fis, I-87036 Arcavacata Di Rende, CS, Italy.
[Escoubet, C. P.] European Space Agcy, Estec, NL-2200 AG Noordwijk, Netherlands.
[Alexandrova, O.] Observ Paris, LESIA, F-92190 Meudon, France.
[Bale, S. D.] Univ Calif Berkeley, Dept Phys, Berkeley, CA 94720 USA.
[Bale, S. D.] Univ Calif Berkeley, Space Sci Lab, Berkeley, CA 94720 USA.
[Balikhin, M.] Univ Sheffield, Dept Automat Control & Syst Engn, Sheffield, S Yorkshire, England.
[Burgessl, D.] Queen Mary Univ London, Sch Phys & Astron, London E1 4NS, England.
[Camporeale, E.] Ctr Math & Comp Sci CWI, NL-1090 GB Amsterdam, Netherlands.
[Caprioli, D.] Princeton Univ, Dept Astrophys Sci, Ivy Lane, Princeton, NJ 08540 USA.
[Chen, C. H. K.; Eastwood, J. P.] Imperial Coll London, Dept Phys, London SW7 2AZ, England.
[Clacey, E.; Rathsman, P.] OHB Sweden, S-16440 Kista, Sweden.
[Cully, C. M.] Univ Calgary, Dept Phys & Astron, Calgary, AB, Canada.
[De Keyser, J.] Belgian Inst Space Aeron, Space Phys Div, Brussels, Belgium.
[Fazakerley, A. N.] Univ Coll London, Mullard Space Sci Lab, Dorking RH5 6NT, Surrey, England.
[Eriksson, S.] Univ Colorado, Lab Atmospher & Space Phys, Boulder, CO 80309 USA.
[Goldstein, M. L.; Moore, T. E.] NASA, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA.
[Haaland, S.] Max Planck Inst Sonnensyst Forsch, D-37077 Gottingen, Germany.
[Haaland, S.] Univ Bergen, Dept Phys & Technol, Bergen, Norway.
[Hoshino, M.] Univ Tokyo, Dept Earth & Planetary Sci, Tokyo, Japan.
[Ji, H.] Princeton Univ, Dept Astrophys Sci, Princeton, NJ 08544 USA.
[Ji, H.] Princeton Univ, Princeton Plasma Phys Lab, Princeton, NJ 08544 USA.
[Karimabadi, H.] SciberQuest, Del Mar, CA 92014 USA.
[Kucharek, H.] Univ New Hampshire, Inst Study Earth Oceans & Space, Durham, NH 03824 USA.
[Lavraud, B.] Univ Toulouse, Inst Rech Astrophys & Planetol, Toulouse, France.
[Lavraud, B.] CNRS, UMR 5277, Toulouse, France.
[Marcucci, F.] INAF IAPS, Rome, Italy.
[Matthaeus, W. H.] Univ Delaware, Bartol Res Inst, Dept Phys & Astron, Newark, DE 19716 USA.
[Nakamura, R.; Narita, Y.; Voeroes, Z.] Austrian Acad Sci, Space Res Inst, Graz, Austria.
[Nemecek, Z.] Charles Univ Prague, Fac Math & Phys, CR-18000 Prague, Czech Republic.
[Palmroth, M.] Finnish Meteorol Inst, Earth Observat Unit, Helsinki, Finland.
[Perrone, D.] ESAC, European Space Agcy, Sci & Robot Explorat Directorate, Madrid, Spain.
[Pinqon, J. -L.] CNRS, LPC2E, Lab Phys & Chim Environm & Espace, Orleans, France.
[Rothkaeh, H.] Polish Acad Sci, Space Res Ctr, Warsaw, Poland.
[Sorriso-Valvo, L.] UOS LICRYL Cosenza, Nanotec CNR, Cubo 31C, I-87036 Arcavacata Di Rende, CS, Italy.
[Vainio, R.] Univ Turku, Dept Phys & Astron, FI-20014 Turku, Finland.
[Wimmer-Schweingruber, R. F.] Univ Kiel, Inst Expt & Appl Phys, Kiel, Germany.
RP Vaivads, A (reprint author), Swedish Inst Space Phys, S-75121 Uppsala, Sweden.
EM andris.vaivads@gmail.com
RI Vainio, Rami/A-5590-2009; Bale, Stuart/E-7533-2011; Soucek,
Jan/G-3424-2014;
OI Vainio, Rami/0000-0002-3298-2067; Bale, Stuart/0000-0002-1989-3596;
Soucek, Jan/0000-0003-0462-6804; Eriksson, Stefan/0000-0002-5619-1577
FU UK Space Agency [ST/N003322/1]; Agenzia Spaziale Italiana [ASI-INAF
2015-039-R.O]; IAPS/INAF, Rome; Belgian Science Policy Office through
PRODEX PEA [4000116805]; Czech Science Foundation [16-04956S]; ESA
PRODEX; CNRS; CNES; German Space Agency [50 00 1603]; Swedish National
Space Board, Uppsala [232/15, 257/15]; Academy of Finland [267144];
European Research Council [682068-PRESTISSIMO, 200141-QuESpace]; ISSI
team 'Kinetic Turbulence and Heating in the Solar wind'; FP7 project
STORM; FP7 project SHOCK; Academy of Finland
FX The THOR science team thanks the Swedish National Space Board for
support to carry out a technical assessment phase study before the
proposal submission. We acknowledge the useful discussion and comments
from the THOR team (http://thor.irfu.se/team) and particularly D.
Delcourt, D. Fontaine, A. Kis, G. Lapenta, M. Maksimovic, M. Opher, G.
Paschmann, A. Petrukovic, S. Schwartz. We acknowledge: the support of
the UK Space Agency through grant ST/N003322/1 to ICL; the support of
Agenzia Spaziale Italiana through contract ASI-INAF 2015-039-R.O to
University of Calabria, Italy and at IAPS/INAF, Rome; the support of the
Belgian Science Policy Office through PRODEX PEA 4000116805 to
BIRA-IASB; the support of the Czech Science Foundation through project
16-04956S to Charles University, Prague; the support of ESA PRODEX to
IAP Prague; the support of CNRS and CNES to IRAP, LPP, LP2CE and LESIA;
the support of the German Space Agency through grant 50 00 1603 to CAU;
the support of Swedish National Space Board through grants 232/15 and
257/15 to IRF, Uppsala; the support of Academy of Finland through grant
267144 and European Research Council Consolidator through grant
682068-PRESTISSIMO to FMI; the support of ISSI team 'Kinetic Turbulence
and Heating in the Solar wind'; the support of FP7 projects STORM and
SHOCK. Vlasiator (http://vlasiator.fmi.fi) has been developed with the
support of Academy of Finland and European Research Council Starting
grant 200141-QuESpace.
NR 28
TC 6
Z9 6
U1 4
U2 4
PU CAMBRIDGE UNIV PRESS
PI NEW YORK
PA 32 AVENUE OF THE AMERICAS, NEW YORK, NY 10013-2473 USA
SN 0022-3778
EI 1469-7807
J9 J PLASMA PHYS
JI J. Plasma Phys.
PD OCT
PY 2016
VL 82
AR 905820501
DI 10.1017/S0022377816000775
PN 5
PG 16
WC Physics, Fluids & Plasmas
SC Physics
GA EF5PZ
UT WOS:000390383400011
ER
PT J
AU Xu, R
Kunz, MW
AF Xu, Rui
Kunz, Matthew W.
TI Linear Vlasov theory of a magnetised, thermally stratified atmosphere
SO JOURNAL OF PLASMA PHYSICS
LA English
DT Article
DE magnetized plasmas; plasma instabilities; space plasma physics
ID GENERAL PLASMA EQUILIBRIA; INTRACLUSTER MEDIUM; MAGNETOROTATIONAL
INSTABILITY; MAGNETOTHERMAL INSTABILITY; BUOYANCY INSTABILITIES; FIELD
CONFIGURATIONS; TRANSPORT-EQUATIONS; GALAXY CLUSTERS; HEAT-TRANSPORT;
DRIVEN
AB The stability of a collisionless, magnetised plasma to local convective disturbances is examined, with a focus on kinetic and finite-Larmor-radius effects. Specific application is made to the outskirts of galaxy clusters, which contain hot and tenuous plasma whose temperature increases in the direction of gravity. At long wavelengths (the 'drift-kinetic' limit), we obtain the kinetic version of the magnetothermal instability (MTI) and its Alfvenic counterpart (Alfvenic MTI), which were previously discovered and analysed using a magnetofluid (i.e. Braginskii) description. At sub-ion-Larmor scales, we discover an overstability driven by the electron-temperature gradient of kinetic-Alfven drift waves - the electron MTI (eMTI) - whose growth rate is even larger than the standard MTI. At intermediate scales, we find that ion finite-Larmor-radius effects tend to stabilise the plasma. We discuss the physical interpretation of these instabilities in detail, and compare them both with previous work on magnetised convection in a collisional plasma and with temperature-gradient-driven drift-wave instabilities well known to the magnetic-confinement-fusion community. The implications of having both fluid and kinetic scales simultaneously driven unstable by the same temperature gradient are briefly discussed.
C1 [Xu, Rui; Kunz, Matthew W.] Princeton Univ, Dept Astrophys Sci, Peyton Hall, Princeton, NJ 08544 USA.
[Kunz, Matthew W.] Princeton Plasma Phys Lab, POB 451, Princeton, NJ 08543 USA.
RP Kunz, MW (reprint author), Princeton Univ, Dept Astrophys Sci, Peyton Hall, Princeton, NJ 08544 USA.; Kunz, MW (reprint author), Princeton Plasma Phys Lab, POB 451, Princeton, NJ 08543 USA.
EM mkunz@princeton.edu
NR 67
TC 0
Z9 0
U1 0
U2 0
PU CAMBRIDGE UNIV PRESS
PI NEW YORK
PA 32 AVENUE OF THE AMERICAS, NEW YORK, NY 10013-2473 USA
SN 0022-3778
EI 1469-7807
J9 J PLASMA PHYS
JI J. Plasma Phys.
PD OCT
PY 2016
VL 82
AR 905820507
DI 10.1017/S0022377816000908
PN 5
PG 54
WC Physics, Fluids & Plasmas
SC Physics
GA EF5PZ
UT WOS:000390383400017
ER
PT J
AU Kumar, S
Kempinski, C
Zhuang, X
Norris, A
Mafu, S
Zi, JC
Bell, SA
Nybo, SE
Kinison, SE
Jiang, ZD
Goklany, S
Linscott, KB
Chen, XL
Jia, QD
Brown, SD
Bowman, JL
Babbitt, PC
Peters, RJ
Chen, F
Chappell, J
AF Kumar, Santosh
Kempinski, Chase
Zhuang, Xun
Norris, Ayla
Mafu, Sibongile
Zi, Jiachen
Bell, Stephen A.
Nybo, Stephen Eric
Kinison, Scott E.
Jiang, Zuodong
Goklany, Sheba
Linscott, Kristin B.
Chen, Xinlu
Jia, Qidong
Brown, Shoshana D.
Bowman, John L.
Babbitt, Patricia C.
Peters, Reuben J.
Chen, Feng
Chappell, Joe
TI Molecular Diversity of Terpene Synthases in the Liverwort Marchantia
polymorpha
SO PLANT CELL
LA English
DT Article
ID ENT-KAURENE SYNTHASE; MOSS PHYSCOMITRELLA-PATENS; BIFUNCTIONAL DITERPENE
CYCLASE; COPALYL DIPHOSPHATE SYNTHASE; FUNCTION LINKAGE DATABASE;
PRE-STEADY-STATE; LAND PLANTS; FUNCTIONAL-CHARACTERIZATION; GIBBERELLIN
BIOSYNTHESIS; NATURAL-PRODUCTS
AB Marchantia polymorpha is a basal terrestrial land plant, which like most liverworts accumulates structurally diverse terpenes believed to serve in deterring disease and herbivory. Previous studies have suggested that the mevalonate and methylerythritol phosphate pathways, present in evolutionarily diverged plants, are also operative in liverworts. However, the genes and enzymes responsible for the chemical diversity of terpenes have yet to be described. In this study, we resorted to a HMMER search tool to identify 17 putative terpene synthase genes from M. polymorpha transcriptomes. Functional characterization identified four diterpene synthase genes phylogenetically related to those found in diverged plants and nine rather unusual monoterpene and sesquiterpene synthase-like genes. The presence of separate monofunctional diterpene synthases for ent-copalyl diphosphate and ent-kaurene biosynthesis is similar to orthologs found in vascular plants, pushing the date of the underlying gene duplication and neofunctionalization of the ancestral diterpene synthase gene family to >400 million years ago. By contrast, the mono-and sesquiterpene synthases represent a distinct class of enzymes, not related to previously described plant terpene synthases and only distantly so to microbial-type terpene synthases. The absence of a Mg2+ binding, aspartate-rich, DDXXD motif places these enzymes in a noncanonical family of terpene synthases.
C1 [Kumar, Santosh; Kempinski, Chase; Zhuang, Xun; Bell, Stephen A.; Nybo, Stephen Eric; Kinison, Scott E.; Jiang, Zuodong; Goklany, Sheba; Linscott, Kristin B.; Chappell, Joe] Univ Kentucky, Plant Biol Program, Lexington, KY 40536 USA.
[Kumar, Santosh; Kempinski, Chase; Zhuang, Xun; Bell, Stephen A.; Nybo, Stephen Eric; Kinison, Scott E.; Jiang, Zuodong; Goklany, Sheba; Linscott, Kristin B.; Chappell, Joe] Univ Kentucky, Dept Pharmaceut Sci, Lexington, KY 40536 USA.
[Norris, Ayla; Jia, Qidong; Chen, Feng] Univ Tennessee, Gradaute Sch Genome Sci & Technol, Knoxville, TN 37996 USA.
[Mafu, Sibongile; Zi, Jiachen; Peters, Reuben J.] Iowa State Univ, Roy J Carver Dept Biochem Biophys & Mol Biol, Ames, IA 50011 USA.
[Chen, Xinlu; Chen, Feng] Univ Tennessee, Dept Plant Sci, Knoxville, TN 37996 USA.
[Brown, Shoshana D.; Babbitt, Patricia C.] Univ Calif San Francisco, Calif Inst Quantitat Biosci, Dept Bioengn, San Francisco, CA 94158 USA.
[Brown, Shoshana D.; Babbitt, Patricia C.] Univ Calif San Francisco, Calif Inst Quantitat Biosci, Dept Therapeut Sci & Pharmaceut Chem, San Francisco, CA 94158 USA.
[Bowman, John L.] Monash Univ, Sch Biol Sci, Melbourne, Vic 3800, Australia.
[Zhuang, Xun] Sandia Natl Labs, Livermore, CA 94551 USA.
[Norris, Ayla] USDA ARS, Crops Pathol & Genet Res Unit, Davis, CA 95616 USA.
[Mafu, Sibongile] Univ Calif Davis, Dept Plant Biol, Davis, CA 95616 USA.
[Zi, Jiachen] Jinan Univ, Biotechnol Inst Chinese Mat Med, Guangzhou 510632, Guangdong, Peoples R China.
[Bell, Stephen A.] Univ Utah, Dept Med Chem, Salt Lake City, UT 84112 USA.
[Nybo, Stephen Eric] Ferris State Univ, Med Chem, Coll Pharm, Big Rapids, MI 49307 USA.
[Goklany, Sheba] Arizona State Univ, Sch Engn Matter Transport & Energy, Tempe, AZ 85287 USA.
RP Chappell, J (reprint author), Univ Kentucky, Plant Biol Program, Lexington, KY 40536 USA.; Chappell, J (reprint author), Univ Kentucky, Dept Pharmaceut Sci, Lexington, KY 40536 USA.
EM chappell@uky.edu
RI Peters, Reuben/D-1196-2010;
OI Peters, Reuben/0000-0003-4691-8477; Chen, Xinlu/0000-0002-7560-6125
FU National Institutes of Health [1RC2GM092521, GM076324, GM60595];
University of Tennessee Institute of Agriculture; Australian Research
Council [DP160100892]; Office of Science of the U.S. Department of
Energy [DE-AC02-05CH11231]
FX We thank Tobias G. Kollner and Jonathan Gershenzon for their
contributions in the early stage of this study. This work was supported,
in part, by Grants 1RC2GM092521 from the National Institutes of Health
to JC, GM076324 from the National Institutes of Health to RJP, an
Innovation Grant from the University of Tennessee Institute of
Agriculture to F.C., GM60595 from the National Institutes of Health to
P.C.B., and DP160100892 from the Australian Research Council to J.L.B.
We also thank our colleagues at Joint Genome Institute for access to the
M. polymorpha genome sequence information, work conducted by the U.S.
Department of Energy Joint Genome Institute, a DOE Office of Science
User Facility, supported by the Office of Science of the U.S. Department
of Energy under Contract DE-AC02-05CH11231.
NR 88
TC 0
Z9 0
U1 13
U2 13
PU AMER SOC PLANT BIOLOGISTS
PI ROCKVILLE
PA 15501 MONONA DRIVE, ROCKVILLE, MD 20855 USA
SN 1040-4651
EI 1532-298X
J9 PLANT CELL
JI Plant Cell
PD OCT
PY 2016
VL 28
IS 10
BP 2632
EP 2650
DI 10.1105/tpc.16.00062
PG 19
WC Biochemistry & Molecular Biology; Plant Sciences; Cell Biology
SC Biochemistry & Molecular Biology; Plant Sciences; Cell Biology
GA EF2DR
UT WOS:000390135400024
PM 27650333
ER
PT J
AU Turner, BL
Tidwell, V
Fernald, A
Rivera, JA
Rodriguez, S
Guldan, S
Ochoa, C
Hurd, B
Boykin, K
Cibils, A
AF Turner, Benjamin L.
Tidwell, Vincent
Fernald, Alexander
Rivera, Jose A.
Rodriguez, Sylvia
Guldan, Steven
Ochoa, Carlos
Hurd, Brian
Boykin, Kenneth
Cibils, Andres
TI Modeling Acequia Irrigation Systems Using System Dynamics: Model
Development, Evaluation, and Sensitivity Analyses to Investigate Effects
of Socio-Economic and Biophysical Feedbacks
SO SUSTAINABILITY
LA English
DT Article
DE acequia irrigation; community sustainability; system dynamics; coupled
natural-human systems; connected hydrologic-human systems; dynamic
hypothesis; leverage points; model development; sensitivity analysis
ID WATER-GROUNDWATER INTERACTIONS; RIVER-BASIN; SIMULATION; ENVIRONMENT;
VALIDATION; MANAGEMENT
AB Agriculture-based irrigation communities of northern New Mexico have survived for centuries despite the arid environment in which they reside. These irrigation communities are threatened by regional population growth, urbanization, a changing demographic profile, economic development, climate change, and other factors. Within this context, we investigated the extent to which community resource management practices centering on shared resources (e.g., water for agricultural in the floodplains and grazing resources in the uplands) and mutualism (i.e., shared responsibility of local residents to maintaining traditional irrigation policies and upholding cultural and spiritual observances) embedded within the community structure influence acequia function. We used a system dynamics modeling approach as an interdisciplinary platform to integrate these systems, specifically the relationship between community structure and resource management. In this paper we describe the background and context of acequia communities in northern New Mexico and the challenges they face. We formulate a Dynamic Hypothesis capturing the endogenous feedbacks driving acequia community vitality. Development of the model centered on major stock-and-flow components, including linkages for hydrology, ecology, community, and economics. Calibration metrics were used for model evaluation, including statistical correlation of observed and predicted values and Theil inequality statistics. Results indicated that the model reproduced trends exhibited by the observed system. Sensitivity analyses of socio-cultural processes identified absentee decisions, cumulative income effect on time in agriculture, and land use preference due to time allocation, community demographic effect, effect of employment on participation, and farm size effect as key determinants of system behavior and response. Sensitivity analyses of biophysical parameters revealed that several key parameters (e.g., acres per animal unit or percentage of normal acequia ditch seepage) which created less variable system responses but which utilized similar pathways to that of the socio-cultural processes (e.g., socio-cultural or physical parameter change ! agricultural profit ! time in spent in agriculture ! effect on socio-cultural or physical processes). These processes also linked through acequia mutualism to create the greatest variability in system outputs compared to the remainder of tests. Results also point to the important role of community mutualism in sustaining linkages between natural and human systems that increase resilience to stressors. Future work will explore scenario development and testing, integration with upland and downstream models, and comparative analyses between acequia communities with distinct social and landscape characteristics.
C1 [Turner, Benjamin L.] Texas A&M Univ Kingsville, Dick & Mary Lewis Coll Agr Nat Resources & Human, 700 Univ Blvd,MSC 228, Kingsville, TX 78363 USA.
[Tidwell, Vincent] Sandia Natl Labs, POB 5800, Albuquerque, NM 87185 USA.
[Fernald, Alexander; Hurd, Brian; Boykin, Kenneth; Cibils, Andres] New Mexico State Univ, Coll Agr Consumer & Environm Sci, POB 30003,MSC 3-1, Las Cruces, NM 88003 USA.
[Rivera, Jose A.] Ctr Reg Studies, MSC05 3020,1 Univ New Mexico, Albuquerque, NM 87131 USA.
[Rodriguez, Sylvia] Dept Anthropol, MSC01-1040,1 Univ New Mexico, Albuquerque, NM 87131 USA.
[Guldan, Steven] New Mexico State Univ, Sustainable Agr Sci Ctr Alcalde, 371 Cty Rd 40,POB 159, Alcalde, NM 87511 USA.
[Ochoa, Carlos] Oregon State Univ, Dept Anim & Rangeland Sci, 124 Withycombe Hall, Corvallis, OR 97331 USA.
RP Turner, BL (reprint author), Texas A&M Univ Kingsville, Dick & Mary Lewis Coll Agr Nat Resources & Human, 700 Univ Blvd,MSC 228, Kingsville, TX 78363 USA.
EM benjamin.turner@tamuk.edu; vctidwe@sandia.gov; afernald@nmsu.edu;
jrivera@unm.edu; sylrodri@unm.edu; sguldan@nmsu.edu;
carlos.ochoa@oregonstate.edu; bhurd@nmsu.edu; kboykin@nmsu.edu;
acibils@nmsu.edu
OI Ochoa, Carlos/0000-0002-4958-919X
FU National Science Foundation's Program on the Dynamics of Coupled Natural
Human Systems [1010516]; New Mexico State University Agricultural
Experiment Station
FX This project was funded by the National Science Foundation's Program on
the Dynamics of Coupled Natural & Human Systems; grant #1010516. General
support was also provided by the New Mexico State University
Agricultural Experiment Station. We also thank three anonymous reviewers
for their helpful comments and suggestions of the manuscript.
NR 55
TC 1
Z9 1
U1 7
U2 7
PU MDPI AG
PI BASEL
PA ST ALBAN-ANLAGE 66, CH-4052 BASEL, SWITZERLAND
SN 2071-1050
J9 SUSTAINABILITY-BASEL
JI Sustainability
PD OCT
PY 2016
VL 8
IS 10
AR 1019
DI 10.3390/su8101019
PG 30
WC GREEN & SUSTAINABLE SCIENCE & TECHNOLOGY; Environmental Sciences;
Environmental Studies
SC Science & Technology - Other Topics; Environmental Sciences & Ecology
GA EE1BE
UT WOS:000389314600059
ER
PT J
AU Tang, WS
Yoshida, K
Soloninin, AV
Skoryunov, RV
Babanova, OA
Skripov, AV
Dimitrievska, M
Stavila, V
Orimo, S
Udovic, TJ
AF Tang, Wan Si
Yoshida, Koji
Soloninin, Alexei V.
Skoryunov, Roman V.
Babanova, Olga A.
Skripov, Alexander V.
Dimitrievska, Mirjana
Stavila, Vitalie
Orimo, Shin-ichi
Udovic, Terrence J.
TI Stabilizing Superionic-Conducting Structures via Mixed-Anion Solid
Solutions of Monocarba-closo-borate Salts
SO ACS ENERGY LETTERS
LA English
DT Article
ID ELECTROLYTES; LITHIUM; TEMPERATURE; DIFFUSION; LI2B12H12; NA2B12H12;
CATION
AB Solid lithium and sodium closo-polyborate-based salts are capable of superionic conductivities surpassing even liquid electrolytes, but often only at above-ambient temperatures where their entropically driven disordered phases become stabilized. Here we show by X-ray diffraction, quasielastic neutron scattering, differential scanning calorimetry, NMR, and AC impedance measurements that by introducing "geometric frustration" via the mixing of two different closo-polyborate anions, namely, 1-CB9H10- and CB11H12-, to form solid-solution anion-alloy salts of lithium or sodium, we can successfully suppress the formation of possible ordered phases in favor of disordered, fast-ion-conducting alloy phases over a broad temperature range from subambient to high temperatures. This result exemplifies an important advancement for further improving on the remarkable conductive properties generally displayed by this class of materials and represents a practical strategy for creating tailored, ambient-temperature, solid, superionic conductors for a variety of upcoming all solid-state energy devices of the future.
C1 [Tang, Wan Si; Dimitrievska, Mirjana; Udovic, Terrence J.] NIST, NIST Ctr Neutron Res, Gaithersburg, MD 20899 USA.
[Tang, Wan Si] Univ Maryland, Dept Mat Sci & Engn, College Pk, MD 20742 USA.
[Yoshida, Koji; Orimo, Shin-ichi] Tohoku Univ, Inst Mat Res, Sendai, Miyagi 9808577, Japan.
[Soloninin, Alexei V.; Skoryunov, Roman V.; Babanova, Olga A.; Skripov, Alexander V.] Russian Acad Sci, Ural Branch, Inst Met Phys, Ekaterinburg 620990, Russia.
[Dimitrievska, Mirjana] Natl Renewable Energy Lab, Golden, CO 80401 USA.
[Stavila, Vitalie] Sandia Natl Labs, Energy Nanomat, Livermore, CA 94551 USA.
[Orimo, Shin-ichi] Tohoku Univ, WPI Adv Inst Mat Res, Sendai, Miyagi 9808577, Japan.
RP Tang, WS; Udovic, TJ (reprint author), NIST, NIST Ctr Neutron Res, Gaithersburg, MD 20899 USA.; Tang, WS (reprint author), Univ Maryland, Dept Mat Sci & Engn, College Pk, MD 20742 USA.; Orimo, S (reprint author), Tohoku Univ, Inst Mat Res, Sendai, Miyagi 9808577, Japan.; Orimo, S (reprint author), Tohoku Univ, WPI Adv Inst Mat Res, Sendai, Miyagi 9808577, Japan.
EM wansi.tang@nist.gov; orimo@imr.tohoku.ac.jp; udovic@nist.gov
RI ORIMO, Shin-ichi/A-4971-2011; Babanova, Olga/J-4821-2013; Skripov,
Alexander/K-4525-2013; Soloninin, Alexey/J-8580-2013;
OI ORIMO, Shin-ichi/0000-0002-4216-0446; Babanova,
Olga/0000-0002-2422-3263; Skripov, Alexander/0000-0002-0610-5538;
Soloninin, Alexey/0000-0001-7127-9641; Skoryunov,
Roman/0000-0001-6158-9056
FU Collaborative Research Center on Energy Materials, Tohoku University;
JSPS KAKENHI [25220911, 26820311]; Russian Federal Agency of Scientific
Organizations [01201463330]; Russian Foundation for Basic Research
[15-03-01114]; U.S. DOE Office of Energy Efficiency and Renewable
Energy, Fuel Cell Technologies Office [DE-AC36-08GO28308]; U.S. DOE's
National Nuclear Security Administration [DE-AC04-94AL85000]; National
Science Foundation [DMR-0944772]
FX This work was performed, in part, in collaboration between members of
IEA HIA Task 32-Hydrogen-based Energy Storage. The authors gratefully
acknowledge support from the Collaborative Research Center on Energy
Materials, Tohoku University; JSPS KAKENHI under Grant Nos. 25220911 and
26820311; the Russian Federal Agency of Scientific Organizations under
Program "Spin" No. 01201463330; and the Russian Foundation for Basic
Research under Grant No. 15-03-01114. M.D. gratefully acknowledges
research support from the U.S. DOE Office of Energy Efficiency and
Renewable Energy, Fuel Cell Technologies Office, under Contract No.
DE-AC36-08GO28308. Sandia National Laboratories is a multiprogram
laboratory managed and operated by Sandia Corporation, a wholly owned
subsidiary of Lockheed Martin Corporation, for the U.S. DOE's National
Nuclear Security Administration under Contract No. DE-AC04-94AL85000.
This work utilized facilities supported in part by the National Science
Foundation under Agreement DMR-0944772.
NR 23
TC 5
Z9 5
U1 6
U2 6
PU AMER CHEMICAL SOC
PI WASHINGTON
PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA
SN 2380-8195
J9 ACS ENERGY LETT
JI ACS Energy Lett.
PD OCT
PY 2016
VL 1
IS 4
BP 659
EP 664
DI 10.1021/acsenergylett.6b00310
PG 6
WC Chemistry, Physical; Electrochemistry; Energy & Fuels; Nanoscience &
Nanotechnology; Materials Science, Multidisciplinary
SC Chemistry; Electrochemistry; Energy & Fuels; Science & Technology -
Other Topics; Materials Science
GA EE5BT
UT WOS:000389620400010
ER
PT J
AU Lindley, BM
Appel, AM
Krogh-Jespersen, K
Mayer, JM
Miller, AJM
AF Lindley, Brian M.
Appel, Aaron M.
Krogh-Jespersen, Karsten
Mayer, James M.
Miller, Alexander J. M.
TI Evaluating the Thermodynamics of Electrocatalytic N-2 Reduction in
Acetonitrile
SO ACS ENERGY LETTERS
LA English
DT Article
ID ELECTRODE-POTENTIALS; AMMONIA-SYNTHESIS; CATALYTIC FORMATION; HYDROGEN
EVOLUTION; NITROGEN-FIXATION; CARBON-DIOXIDE; PINCER LIGAND; SCHROCK
CYCLE; DINITROGEN; CONVERSION
AB The development of a sustainable ammonia synthesis by proton-coupled electroreduction of dinitrogen (N-2) requires knowledge of the thermodynamics described by standard reduction potentials. The first collection of N-2 reduction standard potentials in an organic solvent are reported here. The potentials for reduction of N-2 to ammonia (NH3), hydrazine (N2H4), and diazene (N2H2) in acetonitrile (MeCN) solution are derived using thermochemical cycles. Ammonia is thermodynamically favored, with a 0.43 V difference between NH3 and N2H4 and a 1.26 V difference between NH3 and N2H2. The thermodynamics for reduction of N-2 to the protonated products ammonium (NH4+) and hydrazinium (N2H5+) under acidic conditions are also presented. Comparison with the H+/H-2 potential in MeCN reveals a 63 mV thermodynamic preference for N-2 reduction to NH3 over H-2 production. Combined with knowledge of the kinetics of electrode-catalyzed H-2 evolution, a wide working region is identified to guide future electrocatalytic studies.
C1 [Lindley, Brian M.; Miller, Alexander J. M.] Univ North Carolina Chapel Hill, Dept Chem, Chapel Hill, NC 27599 USA.
[Appel, Aaron M.] Pacific Northwest Natl Lab, Catalysis Sci Grp, Richland, WA 99352 USA.
[Krogh-Jespersen, Karsten] Rutgers State Univ, Dept Chem & Chem Biol, New Brunswick, NJ 08903 USA.
[Mayer, James M.] Yale Univ, Dept Chem, New Haven, CT 06520 USA.
RP Miller, AJM (reprint author), Univ North Carolina Chapel Hill, Dept Chem, Chapel Hill, NC 27599 USA.
EM ajmm@email.unc.edu
OI Appel, Aaron/0000-0002-5604-1253
FU NSF Center for Enabling New Technologies through Catalysis (CENTC)
[CHE-1205189]; Center for Molecular Electrocatalysis, an Energy Frontier
Research Center - U.S. Department of Energy, Office of Science, Office
of Basic Energy Sciences
FX B.M.L., K.K.-J., J.M.M., and A.J.M.M. gratefully acknowledge support
from the NSF Center for Enabling New Technologies through Catalysis
(CENTC), CHE-1205189. For A.M.A., this research was supported as part of
the Center for Molecular Electrocatalysis, an Energy Frontier Research
Center funded by the U.S. Department of Energy, Office of Science,
Office of Basic Energy Sciences. Pacific Northwest National Laboratory
is operated by Battelle for the U.S. Department of Energy.
NR 59
TC 0
Z9 0
U1 16
U2 16
PU AMER CHEMICAL SOC
PI WASHINGTON
PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA
SN 2380-8195
J9 ACS ENERGY LETT
JI ACS Energy Lett.
PD OCT
PY 2016
VL 1
IS 4
BP 698
EP 704
DI 10.1021/acsenergylett.6b00319
PG 7
WC Chemistry, Physical; Electrochemistry; Energy & Fuels; Nanoscience &
Nanotechnology; Materials Science, Multidisciplinary
SC Chemistry; Electrochemistry; Energy & Fuels; Science & Technology -
Other Topics; Materials Science
GA EE5BT
UT WOS:000389620400015
ER
PT J
AU Wei, XL
Duan, WT
Huang, JH
Zhang, L
Li, B
Reed, D
Xu, W
Sprenkle, V
Wang, W
AF Wei, Xiaoliang
Duan, Wentao
Huang, Jinhua
Zhang, Lu
Li, Bin
Reed, David
Xu, Wu
Sprenkle, Vincent
Wang, Wei
TI A High-Current, Stable Nonaqueous Organic Redox Flow Battery
SO ACS ENERGY LETTERS
LA English
DT Article
ID ELECTRICAL ENERGY-STORAGE; ELECTROCHEMICAL PROPERTIES; METAL-FREE;
ELECTROLYTE; PERFORMANCE; SEPARATORS; OPTIMIZATION; CHEMISTRY; PROGRESS;
COUPLES
AB Nonaqueous redox flow batteries are promising in pursuit of high energy density storage systems owing to the broad voltage windows (>2 V) but currently are facing key challenges such as limited cyclability and rate performance. To address these technical hurdles, here we report the nonaqueous organic flow battery chemistry based on N-methylphthalimide anolyte and 2,S-di-tert-butyl-l-methoxy-4-[2'-methoxyethoxy]benzene catholyte, which harvests a theoretical cell voltage of 2.30 V. The redox flow chemistry exhibits excellent cycling stability under both cyclic voltammetry and flow cell tests upon repeated cycling. A series of Daramic and Celgard porous separators are evaluated in this organic flow battery, which enable the cells to be operated at greatly improved current densities as high as 50 mA cm(-2) compared to those of other nonaqueous flow systems. The stable cyclability and high current operations of the organic flow battery system represent significant progress in the development of promising nonaqueous flow batteries.
C1 [Wei, Xiaoliang; Duan, Wentao; Li, Bin; Reed, David; Xu, Wu; Sprenkle, Vincent; Wang, Wei] Pacific Northwest Natl Lab, 902 Battelle Blvd, Richland, WA 99352 USA.
[Huang, Jinhua; Zhang, Lu] Argonne Natl Lab, 9700 South Cass Ave, Argonne, IL 60439 USA.
[Wei, Xiaoliang; Duan, Wentao; Huang, Jinhua; Zhang, Lu] Joint Ctr Energy Storage Res, Argonne, IL 60439 USA.
RP Wei, XL; Wang, W (reprint author), Pacific Northwest Natl Lab, 902 Battelle Blvd, Richland, WA 99352 USA.; Wei, XL (reprint author), Joint Ctr Energy Storage Res, Argonne, IL 60439 USA.
EM Xiaoliang.Wei@pnnl.gov; Wei.Wang@pnnl.gov
RI Wang, Wei/F-4196-2010
OI Wang, Wei/0000-0002-5453-4695
FU U.S. Department of Energy's (DOE's) Office of Electricity Delivery and
Energy Reliability (OE) [57558]; Joint Center for Energy Storage
Research (JCESR), an Energy Innovation Hub - U.S. Department of Energy,
Office of Science, Basic Energy Sciences; DOE [DE-AC05-76RL01830]
FX This research was financially supported by the U.S. Department of
Energy's (DOE's) Office of Electricity Delivery and Energy Reliability
(OE) under Contract No. 57558 (flow chemistry development and
electrochemistry study) and by the Joint Center for Energy Storage
Research (JCESR), an Energy Innovation Hub funded by the U.S. Department
of Energy, Office of Science, Basic Energy Sciences (synthesis of
DBMMB). PNNL is a multiprogram national laboratory operated by Battelle
for DOE under Contract DE-AC05-76RL01830.
NR 43
TC 0
Z9 0
U1 17
U2 17
PU AMER CHEMICAL SOC
PI WASHINGTON
PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA
SN 2380-8195
J9 ACS ENERGY LETT
JI ACS Energy Lett.
PD OCT
PY 2016
VL 1
IS 4
BP 705
EP 711
DI 10.1021/acsenergylett.6b00255
PG 7
WC Chemistry, Physical; Electrochemistry; Energy & Fuels; Nanoscience &
Nanotechnology; Materials Science, Multidisciplinary
SC Chemistry; Electrochemistry; Energy & Fuels; Science & Technology -
Other Topics; Materials Science
GA EE5BT
UT WOS:000389620400016
ER
PT J
AU Burke, CM
Black, R
Kochetkov, IR
Giordani, V
Addison, D
Nazar, LF
McCloskey, BD
AF Burke, Colin M.
Black, Robert
Kochetkov, Ivan R.
Giordani, Vincent
Addison, Dan
Nazar, Linda F.
McCloskey, Bryan D.
TI Implications of 4 e(-) Oxygen Reduction via Iodide Redox Mediation in
Li-O-2 Batteries
SO ACS ENERGY LETTERS
LA English
DT Article
ID LI-AIR BATTERIES; ETHER-BASED ELECTROLYTES; LIMITATIONS; LI2O2;
STABILITY; CAPACITY; SOLVENTS; CHARGE; ELECTROCHEMISTRY; RECHARGEABILITY
AB The nonaqueous lithium-oxygen (Li-O-2) electrochemistry has garnered significant attention because of its high theoretical specific energy compared to the state-of-the-art lithium-ion battery. The common active nonaqueous Li-O-2 battery cathode electrochemistry is the formation (discharge) and decomposition (charge) of lithium peroxide (Li2O2). Recent reports suggest that the introduction of lithium iodide (LiI) to an ether-based electrolyte containing water at impurity levels induces a 4 e(-) oxygen reduction reaction forming lithium hydroxide (LiOH) potentially mitigating instability issues related to typical Li2O2 formation. We provide quantitative analysis of the influence of LiI and H2O on the electrochemistry in a common Li-O-2 battery employing an ether-based electrolyte and a carbon cathode. We confirm, through numerous quantitative techniques, that the addition of LiI and H2O promotes efficient 4 e(-) oxygen reduction to LiOH on discharge, which is unexpected given that only 2 e(-) oxygen reduction is typically observed at undoped carbon electrodes. Unfortunately, LiOH is not reversibly oxidized to O-2 on charge, where instead a complicated mix of redox shuttling and side reactions is observed.
C1 [Burke, Colin M.; McCloskey, Bryan D.] Univ Calif Berkeley, Dept Chem & Biomol Engn, Berkeley, CA 94720 USA.
[Burke, Colin M.; McCloskey, Bryan D.] Lawrence Berkeley Natl Lab, Energy Storage & Distributed Resources Div, Berkeley, CA 94720 USA.
[Black, Robert; Kochetkov, Ivan R.; Nazar, Linda F.] Univ Waterloo, Dept Chem, Waterloo, ON N2L 3G1, Canada.
[Black, Robert; Kochetkov, Ivan R.; Nazar, Linda F.] Waterloo Inst Nanotechnol, Waterloo, ON N2L 3G1, Canada.
[Giordani, Vincent; Addison, Dan] Liox Power Inc, 129 North Hill Ave, Pasadena, CA 91106 USA.
RP McCloskey, BD (reprint author), Univ Calif Berkeley, Dept Chem & Biomol Engn, Berkeley, CA 94720 USA.; McCloskey, BD (reprint author), Lawrence Berkeley Natl Lab, Energy Storage & Distributed Resources Div, Berkeley, CA 94720 USA.; Nazar, LF (reprint author), Univ Waterloo, Dept Chem, Waterloo, ON N2L 3G1, Canada.; Nazar, LF (reprint author), Waterloo Inst Nanotechnol, Waterloo, ON N2L 3G1, Canada.; Addison, D (reprint author), Liox Power Inc, 129 North Hill Ave, Pasadena, CA 91106 USA.
EM dan@liox.com; lfnazar@uwaterloo.ca; bmcclosk@berkeley.edu
FU U.S. Department of Energy, Energy Efficiency and Renewable Energy
Vehicle Technologies Office [DE-0006869]; Laboratory Directed Research
and Development Program of Lawrence Berkeley National Laboratory under
U.S. Department of Energy [DE-AC02-05CH11231]; NASA Space Technology
Research Fellowship [NNX16AM56H]; NRCan through ECO-EII program; NSERC
through Discovery program; NSERC through Canada Research Chair program
FX Helpful discussions with Prof. Clare Grey are gratefully acknowledged.
C.M.B., B.D.M., V.G., and D.A. gratefully acknowledge support from the
U.S. Department of Energy, Energy Efficiency and Renewable Energy
Vehicle Technologies Office under Award No. DE-0006869, and C.M.B and
B.D.M. acknowledge previous support that enabled this work through the
Laboratory Directed Research and Development Program of Lawrence
Berkeley National Laboratory under U.S. Department of Energy Contract
No. DE-AC02-05CH11231. C.M.B. gratefully acknowledges support from a
NASA Space Technology Research Fellowship under Award No. NNX16AM56H.
L.F.N. is grateful for funding for this work from NRCan through their
ECO-EII program and acknowledges NSERC for partial support through the
Discovery and Canada Research Chair programs.
NR 41
TC 3
Z9 3
U1 22
U2 22
PU AMER CHEMICAL SOC
PI WASHINGTON
PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA
SN 2380-8195
J9 ACS ENERGY LETT
JI ACS Energy Lett.
PD OCT
PY 2016
VL 1
IS 4
BP 747
EP 756
DI 10.1021/acsenergylett.6b00328
PG 10
WC Chemistry, Physical; Electrochemistry; Energy & Fuels; Nanoscience &
Nanotechnology; Materials Science, Multidisciplinary
SC Chemistry; Electrochemistry; Energy & Fuels; Science & Technology -
Other Topics; Materials Science
GA EE5BT
UT WOS:000389620400022
ER
PT J
AU Fu, SF
Zhu, CZ
Song, JH
Engelhard, MH
Li, XL
Du, D
Lin, YH
AF Fu, Shaofang
Zhu, Chengzhou
Song, Junhua
Engelhard, Mark H.
Li, Xiaolin
Du, Dan
Lin, Yuehe
TI Highly Ordered Mesoporous Bimetallic Phosphides as Efficient Oxygen
Evolution Electrocatalysts
SO ACS ENERGY LETTERS
LA English
DT Article
ID WATER OXIDATION; HYDROGEN EVOLUTION; COBALT OXIDE; ALKALINE-SOLUTION;
CARBON NANOTUBES; NANOPARTICLES; ELECTRODE; CATALYSTS; NI; OXYHYDROXIDE
AB Oxygen evolution from water using earth-abundant transition-metal based catalysts is of importance for the commercialization of water electrolyzers. Herein, we report a hard templating method to synthesize transition metal phosphides with uniform shape and size. By virtue of the structural feature, synergistic effects among metals, and the in situ formed active species, the as prepared phosphides with optimized composition present enhanced electrocatalytic performance toward the oxygen evolution reaction in alkaline solution. In detail, the catalyst with optimized composition reaches a current density of 10 mA/cm(2) at a potential of 1.511 V vs a reversible hydrogen electrode, which is much lower than that of a commercial RuO2 catalyst. Our work offers a new strategy to optimize the catalysts for water splitting by controlling the morphology and composition.
C1 [Fu, Shaofang; Zhu, Chengzhou; Song, Junhua; Du, Dan; Lin, Yuehe] Washington State Univ, Sch Mech & Mat Engn, Pullman, WA 99164 USA.
[Engelhard, Mark H.; Lin, Yuehe] Pacific Northwest Natl Lab, Environm Mol Sci Lab, Richland, WA 99354 USA.
[Li, Xiaolin] Pacific Northwest Natl Lab, Energy & Environm Directory, Richland, WA 99354 USA.
RP Zhu, CZ; Lin, YH (reprint author), Washington State Univ, Sch Mech & Mat Engn, Pullman, WA 99164 USA.; Lin, YH (reprint author), Pacific Northwest Natl Lab, Environm Mol Sci Lab, Richland, WA 99354 USA.
EM chengzhou.zhu@wsu.edu; yuehe.lin@wsu.edu
RI FU, SHAOFANG/D-2328-2016
OI FU, SHAOFANG/0000-0002-7871-6573
FU start-up fund of Washington State University; Department of Energy's
Office of Biological and Environmental Research at Pacific Northwest
National Laboratory; DOE by Battelle [DE-AC05-76RL0183]
FX This work was supported by a start-up fund of Washington State
University. We thank the Franceschi Microscopy & Image Center at
Washington State University for TEM measurements. The XPS analysis was
performed using EMSL, a national scientific user facility sponsored by
the Department of Energy's Office of Biological and Environmental
Research and located at Pacific Northwest National Laboratory. PNNL is a
multiprogram national laboratory operated for DOE by Battelle under
Contract DE-AC05-76RL0183.
NR 43
TC 1
Z9 1
U1 32
U2 32
PU AMER CHEMICAL SOC
PI WASHINGTON
PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA
SN 2380-8195
J9 ACS ENERGY LETT
JI ACS Energy Lett.
PD OCT
PY 2016
VL 1
IS 4
BP 792
EP 796
DI 10.1021/acsenergylett.6b00408
PG 5
WC Chemistry, Physical; Electrochemistry; Energy & Fuels; Nanoscience &
Nanotechnology; Materials Science, Multidisciplinary
SC Chemistry; Electrochemistry; Energy & Fuels; Science & Technology -
Other Topics; Materials Science
GA EE5BT
UT WOS:000389620400025
ER
PT J
AU Meyer, TJ
AF Meyer, Thomas J.
TI A Conversation with Tom Meyer
SO ACS ENERGY LETTERS
LA English
DT Editorial Material
C1 [Meyer, Thomas J.] Univ N Carolina, Chem, Chapel Hill, NC 27514 USA.
[Meyer, Thomas J.] Univ N Carolina, Energy Frontier Res Ctr Solar Fuels, Chapel Hill, NC 27514 USA.
[Meyer, Thomas J.] Los Alamos Natl Lab, Strateg Res, Los Alamos, NM USA.
[Meyer, Thomas J.] Natl Acad Sci, Washington, DC 20418 USA.
[Meyer, Thomas J.] Amer Acad Arts & Sci, Cambridge, MA 02138 USA.
RP Meyer, TJ (reprint author), Univ N Carolina, Chem, Chapel Hill, NC 27514 USA.; Meyer, TJ (reprint author), Univ N Carolina, Energy Frontier Res Ctr Solar Fuels, Chapel Hill, NC 27514 USA.; Meyer, TJ (reprint author), Natl Acad Sci, Washington, DC 20418 USA.; Meyer, TJ (reprint author), Amer Acad Arts & Sci, Cambridge, MA 02138 USA.
NR 0
TC 0
Z9 0
U1 0
U2 0
PU AMER CHEMICAL SOC
PI WASHINGTON
PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA
SN 2380-8195
J9 ACS ENERGY LETT
JI ACS Energy Lett.
PD OCT
PY 2016
VL 1
IS 4
BP 870
EP 871
DI 10.1021/acsenergylett.6b00482
PG 2
WC Chemistry, Physical; Electrochemistry; Energy & Fuels; Nanoscience &
Nanotechnology; Materials Science, Multidisciplinary
SC Chemistry; Electrochemistry; Energy & Fuels; Science & Technology -
Other Topics; Materials Science
GA EE5BT
UT WOS:000389620400005
ER
PT J
AU Beecheri, AN
Semonin, OE
Skelton, JM
Frost, JM
Terban, MW
Zhai, H
Alatas, A
Owen, JS
Walsh, A
Billinge, SJL
AF Beecheri, Alexander N.
Semonin, Octavi E.
Skelton, Jonathan M.
Frost, Jarvist M.
Terban, Maxwell W.
Zhai, Haowei
Alatas, Ahmet
Owen, Jonathan S.
Walsh, Aron
Billinge, Simon J. L.
TI Direct Observation of Dynamic Symmetry Breaking above Room Temperature
in Methylammonium Lead Iodide Perovskite
SO ACS ENERGY LETTERS
LA English
DT Article
ID AUGMENTED-WAVE METHOD; HALIDE PEROVSKITES; SOLAR-CELLS;
PHASE-TRANSITIONS; HIGH-PERFORMANCE; ORGANIC CATIONS; SCATTERING;
SPECTROSCOPY; CH3NH3PBI3; CRYSTAL
AB Lead halide perovskites such as methylammonium lead triiodide (CH3NH3PbI3) have outstanding optical and electronic properties for photovoltaic applications, yet a full understanding of how this solution-processable material works so well is currently missing. Previous research has revealed that CH3NH3PbI3 possesses multiple forms of static disorder regardless of preparation method, which is surprising in light of its excellent performance. Using high energy resolution inelastic X-ray (HERIX) scattering, we measure phonon dispersions in CH3NH3PbI3 and find direct evidence for another form of disorder in single crystals: large-amplitude anharmonic zone edge rotational instabilities of the PbI6 octahedra that persist to room temperature and above, left over from structural phase transitions that take place tens to hundreds of degrees below. Phonon calculations show that the orientations of the methylanunonium (CH3NH3+) couple strongly and cooperatively to these modes. The result is a noncentrosymmetric, instantaneous local structure, which we observe in atomic pair distribution function (PDF) measurements. This local symmetry breaking is unobservable by Bragg diffraction but can explain key material properties such as the structural phase sequence, ultralow thermal transport, and large minority charge carrier lifetimes despite moderate carrier mobility. From the PDF we estimate the size of the fluctuating symmetry broken domains to be between 1 and 3 run in diameter.
C1 [Beecheri, Alexander N.; Semonin, Octavi E.; Owen, Jonathan S.] Columbia Univ, Dept Chem, New York, NY 10027 USA.
[Skelton, Jonathan M.; Frost, Jarvist M.; Walsh, Aron] Univ Bath, Dept Chem, Claverton Down, Bath BA2 7AY, Avon, England.
[Terban, Maxwell W.; Zhai, Haowei; Billinge, Simon J. L.] Columbia Univ, Dept Appl Phys & Appl Math, New York, NY 10027 USA.
[Alatas, Ahmet] Argonne Natl Lab, Adv Photon Source, Argonne, IL 60439 USA.
[Billinge, Simon J. L.] Brookhaven Natl Lab, Condensed Matter Phys & Mat Sci Dept, Upton, NY 11973 USA.
RP Billinge, SJL (reprint author), Columbia Univ, Dept Appl Phys & Appl Math, New York, NY 10027 USA.; Billinge, SJL (reprint author), Brookhaven Natl Lab, Condensed Matter Phys & Mat Sci Dept, Upton, NY 11973 USA.
EM sb2896@columbia.edu
RI Walsh, Aron/A-7843-2008
OI Walsh, Aron/0000-0001-5460-7033
FU U.S. National Science Foundation [DMR-1534910]; Center for Precision
Assembly of Superstratic and Superatomic Solids, an NSF MRSEC
[DMR-1420634]; DOE Office of Science by Argonne National Laboratory
[DE-AC02-06CH11357]; DOE Office of Science by Brookhaven National
Laboratory [DE-SC0012704]; EPSRC [EP/L000202, EP/M009580/1,
EP/K016288/1, EP/K004956/1]
FX Work in the Billinge group was funded by the U.S. National Science
Foundation through Grant DMR-1534910. Growth and characterization of
single crystals was supported by the Center for Precision Assembly of
Superstratic and Superatomic Solids, an NSF MRSEC (Award Number
DMR-1420634). This research used resources of the Advanced Photon
Source, a U.S. Department of Energy (DOE) Office of Science User
Facility operated for the DOE Office of Science by Argonne National
Laboratory under Contract No. DE-AC02-06CH11357. X-ray PDF measurements
were conducted on beamline 28-ID-2 of the National Synchrotron Light
Source II, a U.S. Department of Energy (DOE) Office of Science User
Facility operated for the DOE Office of Science by Brookhaven National
Laboratory under Contract No. DE-SC0012704. The work at Bath has been
supported by the EPSRC (Grant Nos. EP/L000202, EP/M009580/1,
EP/K016288/1, and EP/K004956/1), and Federico Brivio is thanked for
preliminary phonon calculations. We are grateful to Soham Banerjee for
assistance with PDF measurements and to Bogdan M. Leu, Daniel W. Paley,
Ayman Said, John Tranquada, and Omer Yaffe for helpful conversations.
NR 55
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U1 12
U2 12
PU AMER CHEMICAL SOC
PI WASHINGTON
PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA
SN 2380-8195
J9 ACS ENERGY LETT
JI ACS Energy Lett.
PD OCT
PY 2016
VL 1
IS 4
BP 880
EP 887
DI 10.1021/acsenergylett.6b00381
PG 8
WC Chemistry, Physical; Electrochemistry; Energy & Fuels; Nanoscience &
Nanotechnology; Materials Science, Multidisciplinary
SC Chemistry; Electrochemistry; Energy & Fuels; Science & Technology -
Other Topics; Materials Science
GA EE5BT
UT WOS:000389620400038
ER
PT J
AU DeBenedictis, EP
Williams, RS
AF DeBenedictis, Erik P.
Williams, R. Stanley
TI Help Wanted: A Modern-Day Turing
SO COMPUTER
LA English
DT Editorial Material
AB The National Strategic Computing Initiative will inevitably produce new computer hardware, but what about software?
C1 [DeBenedictis, Erik P.] Sandia Natl Labs, Nonconvent Comp Technol Dept, Livermore, CA 94550 USA.
[Williams, R. Stanley] Hewlett Packard Labs, Palo Alto, CA USA.
RP DeBenedictis, EP (reprint author), Sandia Natl Labs, Nonconvent Comp Technol Dept, Livermore, CA 94550 USA.
EM epdeben@sandia.gov; stan.williams@hpe.com
RI Williams, R. Stanley/A-8281-2009
OI Williams, R. Stanley/0000-0003-0213-4259
NR 8
TC 0
Z9 0
U1 0
U2 0
PU IEEE COMPUTER SOC
PI LOS ALAMITOS
PA 10662 LOS VAQUEROS CIRCLE, PO BOX 3014, LOS ALAMITOS, CA 90720-1314 USA
SN 0018-9162
EI 1558-0814
J9 COMPUTER
JI Computer
PD OCT
PY 2016
VL 49
IS 10
BP 76
EP 79
PG 4
WC Computer Science, Hardware & Architecture; Computer Science, Software
Engineering
SC Computer Science
GA EA0BI
UT WOS:000386248500010
ER
PT J
AU Marino, SR
Lee, SM
Binkowski, TA
Wang, T
Haagenson, M
Wang, HL
Maiers, M
Spellman, S
van Besien, K
Lee, SJ
Karrison, T
Artz, A
AF Marino, S. R.
Lee, S. M.
Binkowski, T. A.
Wang, T.
Haagenson, M.
Wang, H-L
Maiers, M.
Spellman, S.
van Besien, K.
Lee, S. J.
Karrison, T.
Artz, A.
TI Identification of high-risk amino-acid substitutions in hematopoietic
cell transplantation: a challenging task
SO BONE MARROW TRANSPLANTATION
LA English
DT Article
ID BONE-MARROW-TRANSPLANTATION; HLA CLASS-I; ALLELE MISMATCH COMBINATIONS;
VERSUS-HOST-DISEASE; MOLECULAR-MECHANISM; UNRELATED DONORS; IMPACT;
OUTCOMES; BLOOD; HLA-DPB1
AB Allogeneic hematopoietic cell transplantation (HCT) offers the potential to cure hematologic malignancies. In the absence of an HLA-matched donor, HLA mismatched unrelated donors may be used, although risks of GvHD and treatment-related mortality (TRM) are higher. Identification and avoidance of amino-acid substitution and position types (AASPT) conferring higher risks of TRM and GvHD would potentially improve the success of transplantation from single HLA mismatched unrelated donors. Using random forest and logistic regression analyses, we identified 19 AASPT associated with greater risks for at least one adverse transplant outcome: grade III-IV acute GvHD, TRM, lower disease-free survival or worse overall survival relative to HLA-matched unrelated donors and to other AASPT. When tested in an independent validation cohort of 3530 patients, none of the AASPT from the training set were validated as high risk, however. Review of the literature shows that failure to validate original observations is the rule and not the exception in immunobiology and emphasizes the importance of independent validation before clinical application. Our current data do not support avoiding any specific class I AASPT for unrelated donors. Additional studies should be performed to fully understand the role of AASPT in HCT outcomes.
C1 [Marino, S. R.] Univ Chicago, Med Ctr, Dept Pathol, MC 0006,5841 South Maryland Ave, Chicago, IL 60637 USA.
[Lee, S. M.; Karrison, T.] Univ Chicago, Dept Publ Hlth Sci, Chicago, IL USA.
[Binkowski, T. A.] Argonne Natl Lab, Ctr Struct Genom Infect Dis, 9700 S Cass Ave, Argonne, IL 60439 USA.
[Binkowski, T. A.] Argonne Natl Lab, Midwest Ctr Struct Genom, 9700 S Cass Ave, Argonne, IL 60439 USA.
[Wang, T.; Wang, H-L] Med Coll Wisconsin, Div Biostat, Milwaukee, WI 53226 USA.
[Wang, T.; Wang, H-L; Lee, S. J.] Ctr Int Blood & Marrow Transplant Res, Milwaukee, WI USA.
[Haagenson, M.] Ctr Int Blood & Marrow Transplant Res, Minneapolis, MN USA.
[Maiers, M.; Spellman, S.] Natl Marrow Donor Program, Minneapolis, MN USA.
[van Besien, K.] Weill Cornell Med Coll, Div Hematol, New York, NY USA.
[Lee, S. J.] Fred Hutchinson Canc Res Ctr, 1124 Columbia St, Seattle, WA 98104 USA.
[Artz, A.] Univ Chicago, Med Ctr, Dept Med, Chicago, IL 60637 USA.
RP Marino, SR (reprint author), Univ Chicago, Med Ctr, Dept Pathol, MC 0006,5841 South Maryland Ave, Chicago, IL 60637 USA.
EM smarino@bsd.uchicago.edu
OI Maiers, Martin/0000-0002-0198-2064
FU University of Chicago Cancer Research Center, Chicago, Illinois
[6-33573]; Public Health Service National Cancer Institute (NCI)
[U24-CA076518]; National Heart, Lung and Blood Institute (NHLBI);
National Institute of Allergy and Infectious Diseases (NIAID); NHLBI
[5U10HL069294]; NCI; Health Resources and Services Administration
(HRSA/DHHS) [HHSH250201200016C]; Office of Naval Research
[N00014-13-1-0039, N00014-14-1-0028]; Actinium Pharmaceuticals; Allos
Therapeutics, Inc.; Amgen, Inc.; Anonymous donation to the Medical
College of Wisconsin; Ariad; Be the Match Foundation; Blue Cross and
Blue Shield Association; Celgene Corporation; Chimerix, Inc.; Fred
Hutchinson Cancer Research Center; Fresenius-Biotech North America,
Inc.; Gamida Cell Teva Joint Venture Ltd.; Genentech, Inc.; Gentium SpA;
Genzyme Corporation; GlaxoSmithKline; Health Research, Inc.; Roswell
Park Cancer Institute; HistoGenetics, Inc.; Incyte Corporation; Jeff
Gordon Children's Foundation; Kiadis Pharma; Leukemia & Lymphoma
Society; Medac GmbH; Medical College of Wisconsin; Merck Co, Inc.;
Millennium; Takeda Oncology Co.; Milliman USA, Inc.; Miltenyi Biotec,
Inc.; National Marrow Donor Program; Onyx Pharmaceuticals; Optum
Healthcare Solutions, Inc.; Osiris Therapeutics, Inc.; Otsuka America
Pharmaceutical, Inc.; Perkin Elmer, Inc.; Remedy Informatics; Sanofi US;
Seattle Genetics; Sigma-Tau Pharmaceuticals; Soligenix, Inc.; St.
Baldrick's Foundation; StemCyte; Global Cord Blood Therapeutics Co;
Stemsoft Software, Inc.; Swedish Orphan Biovitrum; Tarix
Pharmaceuticals; TerumoBCT; Teva Neuroscience, Inc.; THERAKOS, Inc.;
University of Minnesota; University of Utah and Wellpoint, Inc.
FX This study was partially supported by the University of Chicago Cancer
Research Center, Chicago, Illinois (Fund-6-33573 to SRM). The CIBMTR is
supported by Public Health Service Grant/Cooperative Agreement
U24-CA076518 from the National Cancer Institute (NCI), the National
Heart, Lung and Blood Institute (NHLBI) and the National Institute of
Allergy and Infectious Diseases (NIAID); a Grant/Cooperative Agreement
5U10HL069294 from NHLBI and NCI; a contract HHSH250201200016C with
Health Resources and Services Administration (HRSA/DHHS); two grants
N00014-13-1-0039 and N00014-14-1-0028 from the Office of Naval Research;
and grants from Actinium Pharmaceuticals; Allos Therapeutics, Inc.;
Amgen, Inc.; Anonymous donation to the Medical College of Wisconsin;
Ariad; Be the Match Foundation; Blue Cross and Blue Shield Association;
Celgene Corporation; Chimerix, Inc.; Fred Hutchinson Cancer Research
Center; Fresenius-Biotech North America, Inc.; Gamida Cell Teva Joint
Venture Ltd.; Genentech, Inc.; Gentium SpA; Genzyme Corporation;
GlaxoSmithKline; Health Research, Inc. Roswell Park Cancer Institute;
HistoGenetics, Inc.; Incyte Corporation; Jeff Gordon Children's
Foundation; Kiadis Pharma; the Leukemia & Lymphoma Society; Medac GmbH;
The Medical College of Wisconsin; Merck & Co, Inc.; Millennium: The
Takeda Oncology Co.; Milliman USA, Inc.; Miltenyi Biotec, Inc.; National
Marrow Donor Program; Onyx Pharmaceuticals; Optum Healthcare Solutions,
Inc.; Osiris Therapeutics, Inc.; Otsuka America Pharmaceutical, Inc.;
Perkin Elmer, Inc.; Remedy Informatics; Sanofi US; Seattle Genetics;
Sigma-Tau Pharmaceuticals; Soligenix, Inc.; St. Baldrick's Foundation;
StemCyte, A Global Cord Blood Therapeutics Co.; Stemsoft Software, Inc.;
Swedish Orphan Biovitrum; Tarix Pharmaceuticals; TerumoBCT; Teva
Neuroscience, Inc.; THERAKOS, Inc.; University of Minnesota; University
of Utah and Wellpoint, Inc. The views expressed in this article do not
reflect the official policy or position of the National Institute of
Health, the Department of the Navy, the Department of Defense, Health
Resources and Services Administration or any other agency of the US
Government.
NR 36
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PU NATURE PUBLISHING GROUP
PI LONDON
PA MACMILLAN BUILDING, 4 CRINAN ST, LONDON N1 9XW, ENGLAND
SN 0268-3369
EI 1476-5365
J9 BONE MARROW TRANSPL
JI Bone Marrow Transplant.
PD OCT
PY 2016
VL 51
IS 10
BP 1342
EP 1349
DI 10.1038/bmt.2016.142
PG 8
WC Biophysics; Oncology; Hematology; Immunology; Transplantation
SC Biophysics; Oncology; Hematology; Immunology; Transplantation
GA DZ3GS
UT WOS:000385733800010
PM 27214075
ER
PT J
AU Gilmore, T
Bonneville, A
Sullivan, C
Kelley, M
Appriou, D
Vermeul, V
White, S
Zhang, F
Bjornstad, B
Cornet, F
Gerst, J
Gupta, N
Hund, G
Horner, J
Last, G
Lanigan, D
Oostrom, M
McNeil, C
Moody, M
Rockhold, M
Elliott, M
Spane, F
Strickland, C
Swartz, L
Thorne, P
Brown, C
Hoffmann, J
Humphreys, K
AF Gilmore, Tyler
Bonneville, Alain
Sullivan, Charlotte
Kelley, Mark
Appriou, Delphine
Vermeul, Vince
White, Signe
Zhang, Fred
Bjornstad, Bruce
Cornet, Francois
Gerst, Jacqueline
Gupta, Neeraj
Hund, Gretchen
Horner, Jake
Last, George
Lanigan, Dave
Oostrom, Mart
McNeil, Caitlin
Moody, Mark
Rockhold, Mark
Elliott, Mike
Spane, Frank
Strickland, Chris
Swartz, Lucy
Thorne, Paul
Brown, Christopher
Hoffmann, Jeffrey
Humphreys, Kenneth
TI Characterization and design of the FutureGen 2.0 carbon storage site
SO INTERNATIONAL JOURNAL OF GREENHOUSE GAS CONTROL
LA English
DT Article
DE CO2 reservoir; Carbon sequestration; Characterization; FutureGen
ID MORGAN COUNTY; CO2 STORAGE; ILLINOIS; USA
AB The objective of the FutureGen 2.0 Project was to demonstrate, at the commercial scale, the technical feasibility of implementing carbon capture and storage in a deep saline formation in Illinois, USA. Over approximately 5 years, the FutureGen Industrial Alliance, Inc. (Alliance) conducted a detailed site selection process and identified a site for carbon sequestration storage in Morgan County, Illinois. A comprehensive geologic and hydrologic characterization of the storage site was conducted and included the collection of seismic data and the drilling and characterization of a stratigraphic borehole.
The characterization data provided critical input for developing a site-specific conceptual model and subsequent numerical modeling simulations. The modeling simulations, coupled with upstream designs of the pipeline and power plant, supported the development of a detailed design that included the injection wells and associated control and monitoring infrastructure. The Alliance used all of these data to develop the required documentation to support the applications for four underground injection control (UIC) permits (one for each proposed well). In August 2014, the U.S. Environmental Protection Agency issued four, first-of-their-kind, Class VI UIC permits for carbon sequestration in the United States to the Alliance. This equated to one permit per planned injection well. The information and data generated under this project have been made publicly available through reports and publications, including this journal and others. (C) 2016 Elsevier Ltd. All rights reserved.
C1 [Gilmore, Tyler; Bonneville, Alain; Sullivan, Charlotte; Appriou, Delphine; Vermeul, Vince; White, Signe; Zhang, Fred; Bjornstad, Bruce; Hund, Gretchen; Horner, Jake; Last, George; Lanigan, Dave; Oostrom, Mart; Rockhold, Mark; Elliott, Mike; Spane, Frank; Strickland, Chris; Thorne, Paul; Brown, Christopher] Pacific Northwest Natl Lab, Richland, WA 99352 USA.
[Gerst, Jacqueline; Gupta, Neeraj; McNeil, Caitlin; Moody, Mark] Battelle Mem Inst, Columbus, OH USA.
[Cornet, Francois] Geostress, Strasbourg, France.
[Hoffmann, Jeffrey] Natl Energy Technol Lab, Pittsburgh, PA USA.
[Swartz, Lucy; Humphreys, Kenneth] Futuregen Ind Alliance Inc, Washington, DC USA.
RP Bonneville, A (reprint author), Pacific Northwest Natl Lab, Richland, WA 99352 USA.
EM alain.bonneville@pnnl.gov
OI Bonneville, Alain/0000-0003-1527-1578; Zhang, Fred/0000-0001-8676-6426
FU U.S. federal from the American Recovery and Reinvestment Act; U.S.
Department of Energy [FE0001882]; FutureGen Industrial Alliance, Inc.
[FE0001882]
FX The FutureGen 2.0 Project was supported by U.S. federal funding from the
American Recovery and Reinvestment Act. The program was implemented
under Cooperative Agreement DE-FE0001882 between the U.S. Department of
Energy and the FutureGen Industrial Alliance, Inc. All the information
generated from this project has been made publicly available through
reports and publications, including this journal and others. The authors
thank an anonymous reviewer for his detailed and constructive comments.
NR 33
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PU ELSEVIER SCI LTD
PI OXFORD
PA THE BOULEVARD, LANGFORD LANE, KIDLINGTON, OXFORD OX5 1GB, OXON, ENGLAND
SN 1750-5836
EI 1878-0148
J9 INT J GREENH GAS CON
JI Int. J. Greenh. Gas Control
PD OCT
PY 2016
VL 53
BP 1
EP 10
DI 10.1016/j.ijggc.2016.07.022
PG 10
WC GREEN & SUSTAINABLE SCIENCE & TECHNOLOGY; Energy & Fuels; Engineering,
Environmental
SC Science & Technology - Other Topics; Energy & Fuels; Engineering
GA DW5ZH
UT WOS:000383725700001
ER
PT J
AU Rinehart, AJ
Dewers, TA
Broome, ST
Eichhubl, P
AF Rinehart, Alex J.
Dewers, Thomas A.
Broome, Scott T.
Eichhubl, Peter
TI Effects of CO2 on mechanical variability and constitutive behavior of
the Lower Tuscaloosa Formation, Cranfield Injection Site, USA
SO INTERNATIONAL JOURNAL OF GREENHOUSE GAS CONTROL
LA English
DT Article
DE Chemo-mechanical coupling; Lower Tuscaloosa formation; Cranfield
injection test; Experimental rock mechanics; Elastic moduli degradation;
Chlorite cement
ID CLAY DIAGENESIS; SANDSTONE RESERVOIR; NORTH-SEA; ROCK; BASIN; FIELD;
MISSISSIPPI; QUALITY; CREEP
AB We characterize geomechanical constitutive behavior of reservoir sandstones at conditions simulating the Cranfield Southeast Regional Carbon Sequestration Partnership injection program. From two cores of Lower Tuscaloosa Formation, three sandstone lithofacies were identified for mechanical testing based on permeability and lithology. These include: chlorite-cemented conglomeratic sandstone (Facies A); quartz-cemented fine sandstone (Facies B); and quartz- and calcite-cemented very fine sandstone (Facies C). We performed a suite of compression tests for each lithofacies at 100 degrees C and pore pressure of 30 MPa, including hydrostatic compression and triaxial tests at several confining pressures. Plugs were saturated with supercritical CO2-saturated brine.
Chemical environment affected the mechanical response of all three lithofacies, which experience initial plastic yielding at stresses far below estimated in situ stress. Measured elastic moduli degradation defines a secondary yield surface coinciding with in situ stress for Facies B and C. Facies A shows measurable volumetric creep strain and a failure envelope below estimates of in situ stress, linked to damage of chlorite cements by acidic pore solutions. The substantial weakening of a particular lithofacies by CO2 demonstrates a possible chemical-mechanical coupling during injection at Cranfield with implications for CO2 injection, reservoir permeability stimulation, and enhanced oil recovery. (C) 2016 The Author(s). Published by Elsevier Ltd.
C1 [Rinehart, Alex J.] New Mexico Bur Geol & Mineral Resource, New Mexico Tech, Aquifer Mapping Program, Socorro, NM 57583 USA.
[Dewers, Thomas A.; Broome, Scott T.] Sandia Natl Labs, Geomech Dept, Albuquerque, NM USA.
[Eichhubl, Peter] Texas Bur Econ Geol, Austin, TX USA.
RP Rinehart, AJ (reprint author), New Mexico Bur Geol & Mineral Resource, New Mexico Tech, Aquifer Mapping Program, Socorro, NM 57583 USA.
EM arinehart@nmbg.nmt.edu
FU Center for Frontiers of Subsurface Energy Security; Energy Frontier
Research Center - U.S. Department of Energy, Office of Science, Office
of Basic Energy Sciences [DE-SC0001114]; U.S. Department of Energy's
National Nuclear Security Administration [DE-AC04-94AL85000]
FX This material work was supported as part of the Center for Frontiers of
Subsurface Energy Security, an Energy Frontier Research Center funded by
the U.S. Department of Energy, Office of Science, Office of Basic Energy
Sciences, under Award Number DE-SC0001114. We thank Dr. Susan Hovorka of
the Gulf Coast Carbon Center at the University of Texas-Austin Bureau of
Economic Geology (BEG), and Denbury Onshore LLC, for permission to
access lower Tuscaloosa core from the Cranfield Unit. James Donnelly and
colleagues from the BEG Austin Core Research Center are thanked for core
handling and for providing core plugs for our mechanical testing. We are
grateful to Xiofeng Chen from the BEG for core hardness testing. Greg
Flint, Perry Barrow, Michael Hileman, Mathew Ingraham and Steven Bauer
are thanked for laboratory support at the Sandia Rock Mechanics
Laboratory. We thank Peter Mozley, Glenn Spinelli, David Holcomb, Gary
Axen and Pania Newell for reviews of an early version of this paper.
Sandia National Laboratories is a multi-program laboratory managed and
operated by Sandia Corporation, a wholly owned subsidiary of Lockheed
Martin Corporation, for the U.S. Department of Energy's National Nuclear
Security Administration under contract DE-AC04-94AL85000.
NR 42
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PU ELSEVIER SCI LTD
PI OXFORD
PA THE BOULEVARD, LANGFORD LANE, KIDLINGTON, OXFORD OX5 1GB, OXON, ENGLAND
SN 1750-5836
EI 1878-0148
J9 INT J GREENH GAS CON
JI Int. J. Greenh. Gas Control
PD OCT
PY 2016
VL 53
BP 305
EP 318
DI 10.1016/j.ijggc.2016.08.013
PG 14
WC GREEN & SUSTAINABLE SCIENCE & TECHNOLOGY; Energy & Fuels; Engineering,
Environmental
SC Science & Technology - Other Topics; Energy & Fuels; Engineering
GA DW5ZH
UT WOS:000383725700030
ER
PT J
AU Wing, S
Johnson, JR
Camporeale, E
Reeves, GD
AF Wing, Simon
Johnson, Jay R.
Camporeale, Enrico
Reeves, Geoffrey D.
TI Information theoretical approach to discovering solar wind drivers of
the outer radiation belt
SO JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS
LA English
DT Article
ID RELATIVISTIC ELECTRONS; GEOSYNCHRONOUS ORBIT; GEOMAGNETIC STORMS; MUTUAL
INFORMATION; PLASMA SHEET; ACCELERATION; MAGNETOSPHERE; PREDICTION;
VELOCITY; SPEED
AB The solar wind-magnetosphere system is nonlinear. The solar wind drivers of geosynchronous electrons with energy range of 1.8-3.5 MeV are investigated using mutual information, conditional mutual information (CMI), and transfer entropy (TE). These information theoretical tools can establish linear and nonlinear relationships as well as information transfer. The information transfer from solar wind velocity (V-sw) to geosynchronous MeV electron flux (J(e)) peaks with a lag time of 2 days. As previously reported, J(e) is anticorrelated with solar wind density (n(sw)) with a lag of 1 day. However, this lag time and anticorrelation can be attributed at least partly to the J(e)(t + 2 days) correlation with V-sw(t) and n(sw)(t + 1 day) anticorrelation with V-sw(t). Analyses of solar wind driving of the magnetosphere need to consider the large lag times, up to 3 days, in the (V-sw, n(sw)) anticorrelation. Using CMI to remove the effects of V-sw, the response of Je to n(sw) is 30% smaller and has a lag time < 24 h, suggesting that the MeV electron loss mechanism due to n(sw) or solar wind dynamic pressure has to start operating in < 24 h. nsw transfers about 36% as much information as V-sw (the primary driver) to J(e). Nonstationarity in the system dynamics is investigated using windowed TE. When the data are ordered according to transfer entropy value, it is possible to understand details of the triangle distribution that has been identified between J(e)(t + 2 days) versus V-sw(t).
C1 [Wing, Simon] Johns Hopkins Univ, Appl Phys Lab, Laurel, MD 20723 USA.
[Johnson, Jay R.] Princeton Univ, Plasma Phys Lab, Princeton, NJ USA.
[Johnson, Jay R.] Andrews Univ, Dept Engn & Comp Sci, Berrien Springs, MI 49104 USA.
[Camporeale, Enrico] Ctr Math & Comp Sci CWI, Amsterdam, Netherlands.
[Reeves, Geoffrey D.] Los Alamos Natl Lab, Space Sci & Applicat Grp, Los Alamos, NM USA.
RP Wing, S (reprint author), Johns Hopkins Univ, Appl Phys Lab, Laurel, MD 20723 USA.
EM simon.wing@jhuapl.edu
OI Camporeale, Enrico/0000-0002-7862-6383; Reeves,
Geoffrey/0000-0002-7985-8098
FU JHU/APL Janney Fellowship; NSF [AGS-1058456, ATM0902730, AGS-1203299];
NASA [NNX13AE12G, NNX15AJ01G, NNX16AQ87G, NNH11AR07I, NNX14AM27G,
NNH14AY20I, NNX16AR10G]; DOE [DE-AC02-09CH11466]
FX All the derived data products in this paper are available upon request
by email (simon.wing@jhuapl.edu). Simon Wing acknowledges support from
JHU/APL Janney Fellowship, NSF grant AGS-1058456, and NASA grants
NNX13AE12G, NNX15AJ01G, NNX16AR10G, and NNX16AQ87G. Jay R. Johnson
acknowledges support from NASA grants NNH11AR07I, NNX14AM27G,
NNH14AY20I, NNX16AR10G, and NNX16AQ87G. NSF grants ATM0902730 and
AGS-1203299, and DOE contract DE-AC02-09CH11466.
NR 74
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PU AMER GEOPHYSICAL UNION
PI WASHINGTON
PA 2000 FLORIDA AVE NW, WASHINGTON, DC 20009 USA
SN 2169-9380
EI 2169-9402
J9 J GEOPHYS RES-SPACE
JI J. Geophys. Res-Space Phys.
PD OCT
PY 2016
VL 121
IS 10
BP 9378
EP 9399
DI 10.1002/2016JA022711
PG 22
WC Astronomy & Astrophysics
SC Astronomy & Astrophysics
GA ED6LA
UT WOS:000388965900006
ER
PT J
AU Sarno-Smith, LK
Liemohn, MW
Skoug, RM
Santolik, O
Morley, SK
Breneman, A
Larsen, BA
Reeves, G
Wygant, JR
Hospodarsky, G
Kletzing, C
Moldwin, MB
Katus, RM
Zou, SS
AF Sarno-Smith, Lois K.
Liemohn, Michael W.
Skoug, Ruth M.
Santolik, Ondrej
Morley, Steven K.
Breneman, Aaron
Larsen, Brian A.
Reeves, Geoff
Wygant, John R.
Hospodarsky, George
Kletzing, Craig
Moldwin, Mark B.
Katus, Roxanne M.
Zou, Shasha
TI Hiss or equatorial noise? Ambiguities in analyzing suprathermal ion
plasma wave resonance
SO JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS
LA English
DT Article
ID VAN ALLEN PROBES; DUCTED PLASMASPHERIC HISS; RADIATION BELT PROTONS;
MAGNETOSONIC WAVES; PARTICLE INTERACTIONS; SPATIOTEMPORAL VARIABILITY;
EARTHS MAGNETOSPHERE; GEOSYNCHRONOUS ORBIT; PROPAGATION ANALYSIS;
MAGNETIC EQUATOR
AB Previous studies have shown that low-energy ion heating occurs in the magnetosphere due to strong equatorial noise emission. Observations from the Van Allen Probes Helium Oxygen Proton Electron (HOPE) instrument recently determined that there was a depletion in the 1-10 eV ion population in the postmidnight sector of Earth during quiet times at L < 3. The diurnal variation of equatorially mirroring 1-10 eV H+ ions at 2 < L < 3 is connected with similar diurnal variation in the electric field component of plasma waves ranging between 150 and 600 Hz. Measurements from the Van Allen Probes Electric and Magnetic Field Instrument Suite and Integrated Science (EMFISIS) data set are used to analyze waves of this frequency in near-Earth space. However, when we examine the polarization of the waves in the 150 to 600 Hz range in the equatorial plane, the majority are right-hand polarized plasmaspheric hiss waves. The 1-10 eV H+ equatorially mirroring population does not interact with right-hand waves, despite a strong statistical relationship suggesting that the two are linked. We present evidence supporting the relationship, both in our own work and the literature, but we ultimately conclude that the 1-10 eV H+ heating is not related to the strong enhancement of 150 to 600 Hz waves.
C1 [Sarno-Smith, Lois K.; Liemohn, Michael W.; Moldwin, Mark B.; Zou, Shasha] Univ Michigan, Dept Climate & Space Sci & Engn, Ann Arbor, MI 48109 USA.
[Skoug, Ruth M.; Morley, Steven K.; Larsen, Brian A.; Reeves, Geoff] Los Alamos Natl Lab, Los Alamos, NM USA.
[Santolik, Ondrej] CAS, Inst Atmospher Phys, Dept Space Phys, Prague, Czech Republic.
[Santolik, Ondrej] Charles Univ Prague, Fac Math & Phys, Prague, Czech Republic.
[Breneman, Aaron; Wygant, John R.] Univ Minnesota Twin Cities, Sch Phys & Astron, Minneapolis, MN USA.
[Hospodarsky, George; Kletzing, Craig] Univ Iowa, Dept Phys & Astron, Iowa City, IA 52242 USA.
[Katus, Roxanne M.] Eastern Michigan Univ, Dept Math, Ypsilanti, MI 48197 USA.
RP Sarno-Smith, LK (reprint author), Univ Michigan, Dept Climate & Space Sci & Engn, Ann Arbor, MI 48109 USA.
EM loisks@umich.edu
RI Zou, Shasha/G-2205-2011; Morley, Steven/A-8321-2008; Santolik,
Ondrej/F-7766-2014;
OI Zou, Shasha/0000-0001-7726-2349; Morley, Steven/0000-0001-8520-0199;
Sarno-Smith, Lois/0000-0002-0964-7607; Reeves,
Geoffrey/0000-0002-7985-8098
FU University of Michigan Rackham Graduate school; NASA; NSF [NWX11AO60G,
NWX144AC02G, AGS-1265651, AGS-1102863]; U.S. Department of Energy; NASA
Van Allen Probes mission [NNG07EK09I]; JHU/APL [921647]; Praemium
Academiae award; [LH14010]; [LH15304]
FX The Michigan coauthors would like to thank the University of Michigan
Rackham Graduate school, NASA, and the NSF for sponsoring this work
under grants NWX11AO60G, NWX144AC02G, AGS-1265651, and AGS-1102863. Work
at Los Alamos National Laboratory was performed under the auspices of
the U.S. Department of Energy, with support from the NASA Van Allen
Probes mission under interagency transfer NNG07EK09I and approved for
public release as LA-UR-16-25767. The research at the University of Iowa
was supported by JHU/APL contract 921647. Data from HOPE and EMFISIS
used to generate figures for this project came from the Van Allen Probes
data center at https://emfisis.physics.uiowa.edu/data/index and
http://rbsp-ect.lanl.gov/. O. Santolik acknowledges support from grants
LH14010, LH15304, and from the Praemium Academiae award.
NR 59
TC 1
Z9 1
U1 1
U2 1
PU AMER GEOPHYSICAL UNION
PI WASHINGTON
PA 2000 FLORIDA AVE NW, WASHINGTON, DC 20009 USA
SN 2169-9380
EI 2169-9402
J9 J GEOPHYS RES-SPACE
JI J. Geophys. Res-Space Phys.
PD OCT
PY 2016
VL 121
IS 10
BP 9619
EP 9631
DI 10.1002/2016JA022975
PG 13
WC Astronomy & Astrophysics
SC Astronomy & Astrophysics
GA ED6LA
UT WOS:000388965900021
ER
PT J
AU Cho, JH
Lee, DY
Noh, SJ
Shin, DK
Hwang, J
Kim, KC
Lee, JJ
Choi, CR
Thaller, S
Skoug, R
AF Cho, J. -H.
Lee, D. -Y.
Noh, S. -J.
Shin, D. -K.
Hwang, J.
Kim, K. -C.
Lee, J. J.
Choi, C. R.
Thaller, S.
Skoug, R.
TI Van Allen Probes observations of electromagnetic ion cyclotron waves
triggered by enhanced solar wind dynamic pressure
SO JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS
LA English
DT Article
ID RELATIVISTIC ELECTRON-PRECIPITATION; EMIC WAVES; ULTRARELATIVISTIC
ELECTRONS; STATISTICAL CHARACTERISTICS; PROTON PRECIPITATION;
PLASMASPHERIC PLUME; SUDDEN IMPULSES; RADIATION BELTS; RECOVERY PHASE;
PC-1 WAVES
AB Magnetospheric compression due to impact of enhanced solar wind dynamic pressure P-dyn has long been considered as one of the generation mechanisms of electromagnetic ion cyclotron (EMIC) waves. With the Van Allen Probe-A observations, we identify three EMIC wave events that are triggered by P-dyn enhancements under prolonged northward interplanetary magnetic field (IMF) quiet time preconditions. They are in contrast to one another in a few aspects. Event 1 occurs in the middle of continuously increasing P-dyn while Van Allen Probe-A is located outside the plasmapause at postmidnight and near the equator (magnetic latitude (MLAT) similar to -3 degrees). Event 2 occurs by a sharp P-dyn pulse impact while Van Allen Probe-A is located inside the plasmapause in the dawn sector and rather away from the equator (MLAT similar to 12 degrees). Event 3 is characterized by amplification of a preexisting EMIC wave by a sharp P-dyn pulse impact while Van Allen Probe-A is located outside the plasmapause at noon and rather away from the equator (MLAT similar to -15 degrees). These three events represent various situations where EMIC waves can be triggered by P-dyn increases. Several common features are also found among the three events. (i) The strongest wave is found just above the He+ gyrofrequency. (ii) The waves are nearly linearly polarized with a rather oblique propagation direction (similar to 28 degrees to similar to 39 degrees on average). (iii) The proton fluxes increase in immediate response to the P-dyn impact, most significantly in tens of keV energy, corresponding to the proton resonant energy. (iv) The temperature anisotropy with T-perpendicular to > T-parallel to is seen in the resonant energy for all the events, although its increase by the P-dyn impact is not necessarily always significant. The last two points (iii) and (iv) may imply that in addition to the temperature anisotropy, the increase of the resonant protons must have played a critical role in triggering the EMIC waves by the enhanced P-dyn impact.
C1 [Cho, J. -H.; Lee, D. -Y.; Noh, S. -J.; Shin, D. -K.; Choi, C. R.] Chungbuk Natl Univ, Dept Astron & Space Sci, Cheongju, South Korea.
[Hwang, J.; Lee, J. J.] Korea Astron & Space Sci Inst, Daejeon, South Korea.
[Kim, K. -C.] Daegu Univ, Coll Educ, Dept Earth Sci Educ, Gyongsan, South Korea.
[Thaller, S.] Univ Minnesota, Sch Phys & Astron, Minneapolis, MN 55455 USA.
[Skoug, R.] Los Alamos Natl Lab, Los Alamos, NM USA.
RP Lee, DY (reprint author), Chungbuk Natl Univ, Dept Astron & Space Sci, Cheongju, South Korea.
EM dylee@chungbuk.ac.kr
FU Korea Astronomy and Space Science Institute under RD program; U.S.
Department of Energy; NASA Van Allen Probes mission
FX This research was supported by the Korea Astronomy and Space Science
Institute under the R&D program supervised by the Ministry of Science,
ICT and Future Planning. Work at Los Alamos was performed under the
auspices of the U.S. Department of Energy, with support from the NASA
Van Allen Probes mission. The Van Allen Probes data used for this paper
can be obtained from the NASA's CDAWeb FTP server,
http://cdaweb.gsfc.nasa.gov, and at the EMFISIS website for the magnetic
field and plasma density data, http://emfisis.physics.uiowa.edu/, and at
the Los Alamos National Laboratory ftp site,
ftp://stevens.lanl.gov/pub/projects/rbsp/rbspa/hope, for the HOPE
particle data. The solar wind data used for this work were obtained at
the NASA's CDAWeb, OMNI FTP server, http://omniweb.gsfc.nasa.gov. The
GOES magnetic field data can be obtained at
ftp://satdat.ngdc.noaa.gov/sem/goes/data/new_avg. The ground geomagnetic
data used in this paper can be obtained at
http://www.bcmt.fr/data_download. php for the station AAE, at the DTU
site (http://www.space.dtu.dk) for the station TDC, and at the USGS site
(http://geomag.usgs.gov) for the station GUA. The THEMIS data analysis
software to calculate the WNA and ellipticity is freely available at the
THEMIS website, http://themis.ssl.berkeley.edu/software.shtml.
NR 66
TC 0
Z9 0
U1 0
U2 0
PU AMER GEOPHYSICAL UNION
PI WASHINGTON
PA 2000 FLORIDA AVE NW, WASHINGTON, DC 20009 USA
SN 2169-9380
EI 2169-9402
J9 J GEOPHYS RES-SPACE
JI J. Geophys. Res-Space Phys.
PD OCT
PY 2016
VL 121
IS 10
BP 9771
EP 9793
DI 10.1002/2016JA022841
PG 23
WC Astronomy & Astrophysics
SC Astronomy & Astrophysics
GA ED6LA
UT WOS:000388965900031
ER
PT J
AU Das, S
Bourell, DL
Babu, SS
AF Das, Suman
Bourell, David L.
Babu, S. S.
TI Metallic materials for 3D printing
SO MRS BULLETIN
LA English
DT Article
ID SCANNING LASER EPITAXY; SECTION COMPONENT REPAIR; SINGLE-CRYSTAL
SUPERALLOY; MECHANICAL-PROPERTIES; MICROSTRUCTURE EVOLUTION; DEPOSITED
TI-6AL-4V; GRAIN-STRUCTURE; TITANIUM-ALLOY; MELTING SLM; BEHAVIOR
AB Three-dimensional (3D) printing of metallic materials involves the layerwise consolidation of feedstock materials in the form of powder, wire, or sheet using various energy sources to form complex shapes. The past two decades have witnessed significant advances in the field, in terms of both technologies and materials for metal 3D printing. This has led to widespread exploration and adoption of the technologies across industry, academia, and R&D organizations. This article presents an overview of the field of metal 3D printing. A brief history of metal 3D printing is followed by an overview of metal 3D printing methods and metallic material systems used in these methods. Microstructure and properties, and their relationship to process parameters are discussed next, followed by current challenges and qualification issues. The article concludes with future trends and a brief description of the invited articles included in this special issue.
C1 [Das, Suman] Georgia Inst Technol, Woodruff Sch Mech Engn, Atlanta, GA 30332 USA.
[Das, Suman] Georgia Inst Technol, Sch Mat Sci & Engn, Atlanta, GA 30332 USA.
[Bourell, David L.] Univ Texas Austin, Mech Engn & Mat Sci & Engn, Austin, TX 78712 USA.
[Babu, S. S.] Univ Tennessee, Dept Mech Aerosp & Biomed Engn, Knoxville, TN USA.
[Babu, S. S.] Univ Tennessee, Dept Mat Sci & Engn, Knoxville, TN 37996 USA.
[Babu, S. S.] Oak Ridge Natl Lab, Oak Ridge, TN USA.
RP Das, S (reprint author), Georgia Inst Technol, Woodruff Sch Mech Engn, Atlanta, GA 30332 USA.; Das, S (reprint author), Georgia Inst Technol, Sch Mat Sci & Engn, Atlanta, GA 30332 USA.
EM sumandas@gatech.edu; dbourell@mail.utexas.edu; sbabu@utk.edu
FU US Department of Energy, Office of Energy Efficiency and Renewable
Energy, Advanced Manufacturing Office [DE-AC05-00OR22725]; UT-Battelle,
LLC; Laboratory Directed Research and Development Program of Oak Ridge
National Laboratory
FX Part of the research was sponsored by the US Department of Energy,
Office of Energy Efficiency and Renewable Energy, Advanced Manufacturing
Office, under Contract DE-AC05-00OR22725 with UT-Battelle, LLC. Research
was also sponsored by the Laboratory Directed Research and Development
Program of Oak Ridge National Laboratory, managed by UT-Battelle, LLC.
The US Government retains and the publisher, by accepting the article
for publication, acknowledges that the US Government retains a
non-exclusive, paid-up, irrevocable, worldwide license to publish or
reproduce the published form of this manuscript, or allow others to do
so, for US Government purposes.
NR 114
TC 1
Z9 1
U1 45
U2 45
PU CAMBRIDGE UNIV PRESS
PI NEW YORK
PA 32 AVENUE OF THE AMERICAS, NEW YORK, NY 10013-2473 USA
SN 0883-7694
EI 1938-1425
J9 MRS BULL
JI MRS Bull.
PD OCT
PY 2016
VL 41
IS 10
BP 729
EP 741
DI 10.1557/mrs.2016.217
PG 13
WC Materials Science, Multidisciplinary; Physics, Applied
SC Materials Science; Physics
GA ED8QK
UT WOS:000389135800008
ER
PT J
AU Ross, FM
Wang, CM
de Jonge, N
AF Ross, Frances M.
Wang, Chongmin
de Jonge, Niels
TI Transmission electron microscopy of specimens and processes in liquids
SO MRS BULLETIN
LA English
DT Article
ID FLUORESCENCE MICROSCOPY; ION BATTERIES; CELLS; GROWTH; NUCLEATION;
SILICON; LITHIUM; PHASE; NANOPARTICLES; SPECTROSCOPY
AB Transmission electron microscopy is a powerful technique for the analysis of solid samples, but it can also be used to image in liquid environments, gaining a unique view of processes and structures in liquids. Here, we describe recent developments in electron microscopy of liquids and discuss applications in several areas. We first describe closed-liquid-cell microscopy with its opportunities for visualizing electrochemical processes. We then discuss imaging of low-vapor-pressure liquids relevant to the operation of rechargeable batteries. Finally, we describe imaging of thick biological materials to obtain information on membrane proteins in intact mammalian cells that cannot be observed classically under dry or frozen conditions. Electron microscopy in liquid environments is developing rapidly and has the potential to solve key problems in materials science, physics, chemistry, and biology.
C1 [Ross, Frances M.] IBM TJ Watson Res Ctr, New York, NY 10022 USA.
[Wang, Chongmin] Pacific Northwest Natl Lab, Environm Mol Sci Lab, Richland, WA 99352 USA.
[de Jonge, Niels] INM Leibniz Inst New Mat, Saarbrucken, Germany.
RP Ross, FM (reprint author), IBM TJ Watson Res Ctr, New York, NY 10022 USA.
EM fmross@us.ibm.com; chongmin.wang@pnnl.gov; niels.dejonge@leibniz-inm.de
RI de Jonge, Niels/B-5677-2008
FU INM; Leibniz Association; Assistant Secretary for Energy Efficiency and
Renewable Energy, Office of Vehicle Technologies of the US Department of
Energy (DOE) [DE-AC02-05CH11231, 6951379]; DOE's Office of Biological
and Environmental Research; PNNL
FX F.M.R. acknowledges R.M. Tromp, A.W. Ellis, and M.C. Reuter for their
collaborations during the development of the closed liquid cell. N.J. is
grateful to D.B. Peckys for biological research and discussions, E. Arzt
for his support through INM, and the Leibniz Association. C.M.W.
acknowledges the support of the Assistant Secretary for Energy
Efficiency and Renewable Energy, Office of Vehicle Technologies of the
US Department of Energy (DOE), Contract No. DE-AC02-05CH11231,
Subcontract No. 6951379, under the Battery Materials Research Program.
Part of the research described here was performed at EMSL, a national
scientific user facility sponsored by the DOE's Office of Biological and
Environmental Research and located at PNNL.
NR 59
TC 0
Z9 0
U1 13
U2 13
PU CAMBRIDGE UNIV PRESS
PI NEW YORK
PA 32 AVENUE OF THE AMERICAS, NEW YORK, NY 10013-2473 USA
SN 0883-7694
EI 1938-1425
J9 MRS BULL
JI MRS Bull.
PD OCT
PY 2016
VL 41
IS 10
BP 791
EP 799
DI 10.1557/mrs.2016.212
PG 9
WC Materials Science, Multidisciplinary; Physics, Applied
SC Materials Science; Physics
GA ED8QK
UT WOS:000389135800016
ER
PT J
AU Kang, YJ
Yang, PD
Markovic, NM
Stamenkovic, VR
AF Kang, Yijin
Yang, Peidong
Markovic, Nenad M.
Stamenkovic, Vojislav R.
TI Shaping electrocatalysis through tailored nanomaterials
SO Nano Today
LA English
DT Review
DE Electrocatalysis; Platinum alloys; Surface modification
ID OXYGEN REDUCTION REACTION; MEMBRANE FUEL-CELLS; HIGH-INDEX FACETS;
COLLOIDAL PLATINUM NANOPARTICLES; NOBLE-METAL NANOPARTICLES;
SINGLE-CRYSTAL SURFACES; SULFURIC-ACID-SOLUTION; ACTIVE EDGE SITES;
FORMIC-ACID; ENHANCED ELECTROCATALYSIS
AB Electrocatalysis is a subclass of heterogeneous catalysis that is aimed towards increase of the electrochemical reaction rates that are taking place at the surface of electrodes. Real-world electrocatalysts are usually based on precious metals in the form of nanoparticles due to their high surface-to-volume ratio, which enables better utilization of employed materials. Ability to tailor nanostructure of an electrocatalyst is critical in order to tune their electrocatalytic properties. Over the last decade, that has mainly been achieved through implementation of fundamental studies performed on well-defined extended surfaces with distinct single crystalline and polycrystalline structures. Based on these studies, it has been demonstrated that performance of an electrocatalyst could be significantly changed through the control of size, composition, morphology and architecture of employed nanomaterials. This review outlines the following steps in the process of rational development of an efficient electrocatalyst: 1) electrochemical properties of well-defined surfaces, 2) synthesis and characterization of different classes of electrocatalysts, and 3) correlation between physical properties (size, shape, composition and morphology) and electrochemical behavior (adsorption, electrocatalytic activity and durability) of electrocatalyst. In addition, this is a brief summary of the novel research platforms in the development of functional nano materials for energy conversion and storage applications such as fuel cells electrolyzers and batteries. (C) 2016 Elsevier Ltd. All rights reserved.
C1 [Kang, Yijin] Univ Elect Sci & Technol China, Inst Fundamental & Frontier Sci, Chengdu, Peoples R China.
[Yang, Peidong] Univ Calif Berkeley, Dept Chem, Berkeley, CA 94720 USA.
[Markovic, Nenad M.; Stamenkovic, Vojislav R.] Argonne Natl Lab, Div Mat Sci, 9700 Cass Ave, Argonne, IL 60439 USA.
RP Stamenkovic, VR (reprint author), Argonne Natl Lab, Div Mat Sci, 9700 Cass Ave, Argonne, IL 60439 USA.
EM vrstamenkovic@anl.gov
FU U.S. Department of Energy, Office of Science, Office of Basic Energy
Sciences, Materials Sciences and Engineering Division
[DE-AC02-06CH11357, DE-AC02-05CH11231]; Office of Energy Efficiency and
Renewable Energy, Fuel Cell Technologies Program
FX The research conducted at Argonne National Laboratory, was supported by
the U.S. Department of Energy, Office of Science, Office of Basic Energy
Sciences, Materials Sciences and Engineering Division, under Contract
No. DE-AC02-06CH11357 and by the Office of Energy Efficiency and
Renewable Energy, Fuel Cell Technologies Program. The portion of the
research conducted at Lawrence Berkeley National Laboratory was
supported by the U.S. Department of Energy, Office of Science, Office of
Basic Energy Sciences, Materials Sciences and Engineering Division,
under Contract No. DE-AC02-05CH11231. The authors thank to Chao Wang,
Joshua Snyder, Dennis van der Vliet, Dusan Strmcnik, Dusan Tripkovic,
Arvydas Paulikas, Jeffrey Greeley, Deborah Myers, Karren More and Philip
Ross for many years of collaboration that has led to a number of
publications in the field of electrocatalysis.
NR 168
TC 0
Z9 0
U1 72
U2 72
PU ELSEVIER SCI LTD
PI OXFORD
PA THE BOULEVARD, LANGFORD LANE, KIDLINGTON, OXFORD OX5 1GB, OXON, ENGLAND
SN 1748-0132
EI 1878-044X
J9 NANO TODAY
JI Nano Today
PD OCT
PY 2016
VL 11
IS 5
BP 587
EP 600
DI 10.1016/j.nantod.2016.08.008
PG 14
WC Chemistry, Multidisciplinary; Nanoscience & Nanotechnology; Materials
Science, Multidisciplinary
SC Chemistry; Science & Technology - Other Topics; Materials Science
GA ED8GC
UT WOS:000389109000009
ER
PT J
AU Zheng, JM
Xiao, J
Zhang, JG
AF Zheng, Jianming
Xiao, Jie
Zhang, Ji-Guang
TI The roles of oxygen non-stoichiometry on the electrochemical properties
of oxide-based cathode materials
SO Nano Today
LA English
DT Review
DE Oxygen non-stoichiometry; Cathode materials; Ni-rich material; High
voltage spinel; Li-rich Mn-rich; Lithium ion battery
ID LITHIUM-ION BATTERIES; LAYERED COMPOSITE CATHODE; VOLTAGE SPINEL
LINI0.5MN1.5O4; NICKEL MANGANESE OXIDES; SITU X-RAY; HIGH-ENERGY;
HIGH-CAPACITY; ELECTRODE MATERIALS; THERMAL-STABILITY; 1ST-PRINCIPLES
CALCULATIONS
AB Cathode materials with both high energy density and high power capability are in great demand to improve the performance of lithium ion batteries and expand the driving range of electric vehicles. Of particular interest are transition metal oxide-based cathodes. However, electrochemical performance of these cathode materials is very sensitive to the synthetic conditions and, particularly, the oxygen non-stoichiometry that is induced during high temperature synthesis and post treatment. This review highlights the critical roles of oxygen non-stoichiometry in high-energy-density cathode materials including high voltage spinet LiNi0.5Mn1.5O4, Ni-rich layered LiNixMnyCozO2 (NMC, x >0.5), and the Li-rich, Mn-rich layered cathode, with the aim to provide a fundamental understanding on the effects of the oxygen non-stoichiometry governing the crystalline structure, electrochemical performance, and thermal stability of different cathode materials. This review also offers perspectives and directions on how to best utilize oxygen non-stoichiometry in the future development of high-energy-density cathode materials for lithium ion batteries. (C) 2016 Elsevier Ltd. All rights reserved.
C1 [Zheng, Jianming; Xiao, Jie; Zhang, Ji-Guang] Pacific Northwest Natl Lab, Energy & Environm Directorate, 902 Battelle Blvd, Richland, WA 99352 USA.
RP Zhang, JG (reprint author), Pacific Northwest Natl Lab, Energy & Environm Directorate, 902 Battelle Blvd, Richland, WA 99352 USA.
EM jiguang.zhang@pnnl.gov
FU Assistant Secretary for Energy Efficiency and Renewable Energy, Office
of Vehicle Technologies of the U.S. Department of Energy
[DE-AC02-05CH11231, 18769]; U.S. Department of Energy's Office of
Biological and Environmental Research
FX This work is supported by the Assistant Secretary for Energy Efficiency
and Renewable Energy, Office of Vehicle Technologies of the U.S.
Department of Energy under Contract No. DE-AC02-05CH11231, Subcontract
No. 18769, under the Advanced Battery Materials Research program. The
authors would like to thank Mr. Mark H. Engelhard for XPS measurements
as shown in Fig. 12, which were conducted in William R. Wiley
Environmental Molecular Sciences Laboratory, a national scientific user
facility sponsored by the U.S. Department of Energy's Office of
Biological and Environmental Research and located at Pacific Northwest
National Laboratory.
NR 128
TC 0
Z9 0
U1 55
U2 55
PU ELSEVIER SCI LTD
PI OXFORD
PA THE BOULEVARD, LANGFORD LANE, KIDLINGTON, OXFORD OX5 1GB, OXON, ENGLAND
SN 1748-0132
EI 1878-044X
J9 NANO TODAY
JI Nano Today
PD OCT
PY 2016
VL 11
IS 5
BP 678
EP 694
DI 10.1016/j.nantod.2016.08.011
PG 17
WC Chemistry, Multidisciplinary; Nanoscience & Nanotechnology; Materials
Science, Multidisciplinary
SC Chemistry; Science & Technology - Other Topics; Materials Science
GA ED8GC
UT WOS:000389109000014
ER
PT J
AU Daly, RA
Borton, MA
Wilkins, MJ
Hoyt, DW
Kountz, DJ
Wolfe, RA
Welch, SA
Marcus, DN
Trexler, RV
MacRae, JD
Krzycki, JA
Cole, DR
Mouser, PJ
Wrighton, KC
AF Daly, Rebecca A.
Borton, Mikayla A.
Wilkins, Michael J.
Hoyt, David W.
Kountz, Duncan J.
Wolfe, Richard A.
Welch, Susan A.
Marcus, Daniel N.
Trexler, Ryan V.
MacRae, Jean D.
Krzycki, Joseph A.
Cole, David R.
Mouser, Paula J.
Wrighton, Kelly C.
TI Microbial metabolisms in a 2.5-km-deep ecosystem created by hydraulic
fracturing in shales
SO Nature Microbiology
LA English
DT Article
ID CRISPR-CAS SYSTEMS; GAS-WELLS; METAGENOMIC DATA; BACTERIAL; WATER; GENE;
CLASSIFICATION; IDENTIFICATION; ENVIRONMENT; EXTRACTION
AB Hydraulic fracturing is the industry standard for extracting hydrocarbons from shale formations. Attention has been paid to the economic benefits and environmental impacts of this process, yet the biogeochemical changes induced in the deep subsurface are poorly understood. Recent single-gene investigations revealed that halotolerant microbial communities were enriched after hydraulic fracturing. Here, the reconstruction of 31 unique genomes coupled to metabolite data from the Marcellus and Utica shales revealed that many of the persisting organisms play roles in methylamine cycling, ultimately supporting methanogenesis in the deep biosphere. Fermentation of injected chemical additives also sustains long-term microbial persistence, while thiosulfate reduction could produce sulfide, contributing to reservoir souring and infrastructure corrosion. Extensive links between viruses and microbial hosts demonstrate active viral predation, which may contribute to the release of labile cellular constituents into the extracellular environment. Our analyses show that hydraulic fracturing provides the organismal and chemical inputs for colonization and persistence in the deep terrestrial subsurface.
C1 [Daly, Rebecca A.; Borton, Mikayla A.; Wilkins, Michael J.; Kountz, Duncan J.; Wolfe, Richard A.; Marcus, Daniel N.; Krzycki, Joseph A.; Wrighton, Kelly C.] Ohio State Univ, Dept Microbiol, Columbus, OH 43214 USA.
[Wilkins, Michael J.; Welch, Susan A.; Cole, David R.] Ohio State Univ, Sch Earth Sci, Columbus, OH 43214 USA.
[Hoyt, David W.] Pacific Northwest Natl Lab, EMSL, Richland, WA 99352 USA.
[Trexler, Ryan V.; Mouser, Paula J.] Ohio State Univ, Dept Civil Environm & Geodet Engn, Columbus, OH 43214 USA.
[MacRae, Jean D.] Univ Maine, Dept Civil & Environm Engn, Orono, ME 04469 USA.
RP Wrighton, KC (reprint author), Ohio State Univ, Dept Microbiol, Columbus, OH 43214 USA.
EM wrighton.1@osu.edu
FU National Sciences Foundation Dimensions of Biodiversity [1342701];
Alfred P. Sloan Foundation; Office of Biological and Environmental
Research [DE-AC02-05CH11231, DE-AC05-76RL01830]
FX M.A.B., D.R.C., R.A.D., D.N.M., P.J.M., R.V.T., S.A.W., M.J.W. and
K.C.W. are partially supported by funding from the National Sciences
Foundation Dimensions of Biodiversity (award no. 1342701). The authors
thank the National Energy Technology Laboratory for access to the
Marcellus samples. The Marcellus Illumina sequencing was made possible
by the Deep Carbon Observatory's Census of Deep Life supported by the
Alfred P. Sloan Foundation (awards to K.C.W and P.J.M.). The authors
also thank members of the Marine Biological Laboratory (MBL) at Woods
Hole, MA, and acknowledge M. Sogin, N. Downey, H. Morrison and J. Vineis
at MBL. Sequencing of the Utica fluid enrichment was conducted at the
OSU Comprehensive Cancer Center, and the authors thank Pearlly Yan in
particular. S. Roux and J. Emerson are thanked for viromics guidance. A
portion of this research was performed under the JGI-EMSL Collaborative
Science Initiative (award to K.C.W.) and used resources at the DOE Joint
Genome Institute and Environmental Molecular Sciences Laboratory, which
are DOE Office of Science User Facilities. Both facilities are sponsored
by the Office of Biological and Environmental Research and operated
under contracts nos. DE-AC02-05CH11231 (JGI) and DE-AC05-76RL01830
(EMSL).
NR 51
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Z9 4
U1 30
U2 30
PU NATURE PUBLISHING GROUP
PI LONDON
PA MACMILLAN BUILDING, 4 CRINAN ST, LONDON N1 9XW, ENGLAND
SN 2058-5276
J9 NAT MICROBIOL
JI NAT. MICROBIOL
PD OCT
PY 2016
VL 1
IS 10
AR 16146
DI 10.1038/NMICROBIOL.2016.146
PG 9
WC Microbiology
SC Microbiology
GA ED8RS
UT WOS:000389139200012
ER
PT J
AU Gionfriddo, CM
Tate, MT
Wick, RR
Schultz, MB
Zemla, A
Thelen, MP
Schofield, R
Krabbenhoft, DP
Holt, KE
Moreau, JW
AF Gionfriddo, Caitlin M.
Tate, Michael T.
Wick, Ryan R.
Schultz, Mark B.
Zemla, Adam
Thelen, Michael P.
Schofield, Robyn
Krabbenhoft, David P.
Holt, Kathryn E.
Moreau, John W.
TI Microbial mercury methylation in Antarctic sea ice
SO Nature Microbiology
LA English
DT Article
ID NITROSPINA-LIKE BACTERIA; FRESH-WATER; INORGANIC MERCURY; SURFACE
WATERS; SOUTHERN-OCEAN; ARCTIC-OCEAN; SNOW; BRINE; METHYLMERCURY;
METAGENOMICS
AB Atmospheric deposition of mercury onto sea ice and circumpolar sea water provides mercury for microbial methylation, and contributes to the bioaccumulation of the potent neurotoxin methylmercury in the marine food web. Little is known about the abiotic and biotic controls on microbial mercury methylation in polar marine systems. However, mercury methylation is known to occur alongside photochemical and microbial mercury reduction and subsequent volatilization. Here, we combine mercury speciation measurements of total and methylated mercury with metagenomic analysis of whole-community microbial DNA from Antarctic snow, brine, sea ice and sea water to elucidate potential microbially mediated mercury methylation and volatilization pathways in polar marine environments. Our results identify the marine microaerophilic bacterium Nitrospina as a potential mercury methylator within sea ice. Anaerobic bacteria known to methylate mercury were notably absent from sea-ice metagenomes. We propose that Antarctic sea ice can harbour a microbial source of methylmercury in the Southern Ocean.
C1 [Gionfriddo, Caitlin M.; Schofield, Robyn; Moreau, John W.] Univ Melbourne, Sch Earth Sci, Parkville, Vic 3010, Australia.
[Tate, Michael T.; Krabbenhoft, David P.] US Geol Survey, Wisconsin Water Sci Ctr, Middleton, WI 53562 USA.
[Wick, Ryan R.; Schultz, Mark B.; Holt, Kathryn E.] Univ Melbourne, Ctr Syst Genom, Melbourne, Vic 3010, Australia.
[Wick, Ryan R.; Schultz, Mark B.; Holt, Kathryn E.] Univ Melbourne, Mol Sci & Biotechnol Inst Bio21, Dept Biochem & Mol Biol, Melbourne, Vic 3010, Australia.
[Zemla, Adam] Lawrence Livermore Natl Lab, Computat Directorate, Livermore, CA 94550 USA.
[Thelen, Michael P.] Lawrence Livermore Natl Lab, Phys & Life Sci Directorate, Livermore, CA 94550 USA.
RP Moreau, JW (reprint author), Univ Melbourne, Sch Earth Sci, Parkville, Vic 3010, Australia.
EM jmoreau@unimelb.edu.au
RI Schofield, Robyn/A-4062-2010;
OI Schofield, Robyn/0000-0002-4230-717X; Gionfriddo,
Caitlin/0000-0003-0745-9255; Schultz, Mark/0000-0002-7689-6531
FU Australian Antarctic Division [AAD4032]; University of Melbourne Joyce
Lambert Antarctic Research Seed Funding Grant [501325]
FX The authors acknowledge funding support from the Australian Antarctic
Division (AAD4032, awarded to R.S., J.W.M., M.T.T. and D.P.K.) and The
University of Melbourne Joyce Lambert Antarctic Research Seed Funding
Grant (no. 501325, awarded to M.B.S., K.E.H. and J.W.M.). The authors
thank K. Meiners for contributions to the sea ice chemistry data and
shipboard logistical support as the Chief Scientist of SIPEX II; A.
Klekociuk (Australian Antarctic Division, Co-Investigator on AAD4032)
for shipboard logistical support; D. Lannuzel and A. Bowie (University
of Tasmania) for making trace metal data available and for shipboard
sampling and logistical support; K. Westwood at the Australian Antarctic
Division for assistance in the biology laboratory and contributions to
water chemistry data; and A. Martin, S. Ugalde, F. Chever, C.
Schallenberg and J. Janssens (SIPEX II Science Party) for logistical
assistance on the ice. The authors also thank J. Banfield and B. Thomas
(University of California-Berkeley) for help with ggKbase. The authors
thank J. Santillan and C. Gilmour (Smithsonian Environmental Research
Center) for their constructive review that helped to improve this
manuscript.
NR 93
TC 2
Z9 2
U1 11
U2 12
PU NATURE PUBLISHING GROUP
PI LONDON
PA MACMILLAN BUILDING, 4 CRINAN ST, LONDON N1 9XW, ENGLAND
SN 2058-5276
J9 NAT MICROBIOL
JI NAT. MICROBIOL
PD OCT
PY 2016
VL 1
IS 10
AR 16127
DI 10.1038/NMICROBIOL.2016.127
PG 12
WC Microbiology
SC Microbiology
GA ED8RS
UT WOS:000389139200004
PM 27670112
ER
PT J
AU Bongi, M
Adriani, O
Bertiah, E
Bonechi, L
Castellini, G
D'Alessandro, R
Del Prete, M
Haguenauer, M
Itow, Y
Iwata, T
Kasahara, K
Kawade, K
Makino, Y
Masuda, K
Matsubara, Y
Matsubayashi, E
Menjo, H
Mitsuka, G
Muraki, Y
Olcuno, Y
Papini, P
Perrot, AL
Ricciarini, S
Sako, T
Sakurai, N
Shimizu, Y
Sugiura, Y
Suzuki, T
Tamura, T
Tiberio, A
Torii, S
Tricomi, A
Turner, WC
Ueno, M
Yoshida, K
Zhou, QD
AF Bongi, M.
Adriani, O.
Bertiah, E.
Bonechi, L.
Castellini, G.
D'Alessandro, R.
Del Prete, M.
Haguenauer, M.
Itow, Y.
Iwata, T.
Kasahara, K.
Kawade, K.
Makino, Y.
Masuda, K.
Matsubara, Y.
Matsubayashi, E.
Menjo, H.
Mitsuka, G.
Muraki, Y.
Olcuno, Y.
Papini, P.
Perrot, A. -L.
Ricciarini, S.
Sako, T.
Sakurai, N.
Shimizu, Y.
Sugiura, Y.
Suzuki, T.
Tamura, T.
Tiberio, A.
Torii, S.
Tricomi, A.
Turner, W. C.
Ueno, M.
Yoshida, K.
Zhou, Q. D.
TI LHCf Experiment: Physics Results
SO NUCLEAR AND PARTICLE PHYSICS PROCEEDINGS
LA English
DT Proceedings Paper
CT 9th Cosmic Ray International Seminar (CRIS)
CY SEP 14-16, 2015
CL Gallipoli, ITALY
SP Univ Salento, Dept Math & Phys E De Giorgi, Ist Nazl Fis Nucleare
DE LHC; Ultra-high energy cosmic-ray; Hadronic interaction models
ID PROTON-PROTON COLLISIONS; PHOTON ENERGY-SPECTRA
AB LHCf is an experiment designed to study the forward emission of neutral particles produced in proton-proton and proton-nucleus collisions at the LHC. The detectors consists of a pair of electromagnetic sampling calorimeters installed on both sides of the ATLAS interaction point IP1 at a distance of 140 m, covering the pseudorapidity range from 8.4 to infinity. The experiment has successfully measured the energy spectra of gamma rays, neutral pions and neutrons in p-p collisions at 0.9 TeV and 7 TeV, and of neutral pions in p-Pb collisions at 5.02 TeV and in p-p collisions at 2.76 TeV. The most recent data set has been acquired during a special physics run of p-p collisions at 13 TeV in June 2015 after the restart of the LHC. This set of measurements represent an useful contribution to the calibration and tuning of the hadronic interaction models used for the simulation of atmospheric showers induced by very-high energy cosmic rays, as the measured energy interval corresponds to the range 10(14) - 10(17) eV in the laboratory frame.
C1 [Bongi, M.; Adriani, O.; Bertiah, E.; Bonechi, L.; Castellini, G.; D'Alessandro, R.; Del Prete, M.; Mitsuka, G.; Papini, P.; Ricciarini, S.; Tiberio, A.] Ist Nazl Fis Nucl, Sect Florence, Florence, Italy.
[Bongi, M.; Adriani, O.; Bertiah, E.; D'Alessandro, R.; Del Prete, M.; Mitsuka, G.; Tiberio, A.] Univ Florence, Florence, Italy.
[Castellini, G.; Ricciarini, S.] CNR, IFAC, Rome, Italy.
[Haguenauer, M.] Ecole Polytech, Palaiseau, France.
[Itow, Y.; Kawade, K.; Makino, Y.; Masuda, K.; Matsubara, Y.; Matsubayashi, E.; Muraki, Y.; Olcuno, Y.; Sako, T.; Sugiura, Y.; Ueno, M.; Zhou, Q. D.] Nagoya Univ, Inst Space Earth Environm Res, Nagoya, Aichi, Japan.
[Itow, Y.; Sako, T.] Nagoya Univ, Kobayashi Maskawa Inst, Nagoya, Aichi, Japan.
[Iwata, T.; Kasahara, K.; Suzuki, T.; Torii, S.] Waseda Univ, Tokyo, Japan.
[Menjo, H.] Nagoya Univ, Grad Sch Sci, Nagoya, Aichi, Japan.
[Perrot, A. -L.] CERN, Geneva, Switzerland.
[Sakurai, N.] Univ Tokushima, Tokushima, Japan.
[Shimizu, Y.; Tamura, T.] Kanagawa Univ, Yokohama, Kanagawa, Japan.
[Tricomi, A.] Ist Nazl Fis Nucl, Sect Catania, Catania, Italy.
[Tricomi, A.] Univ Catania, Catania, Italy.
[Turner, W. C.] LBNL, Berkeley, CA USA.
[Yoshida, K.] Shibaura Inst Technol, Tokyo, Japan.
RP Bongi, M (reprint author), Ist Nazl Fis Nucl, Sect Florence, Florence, Italy.; Bongi, M (reprint author), Univ Florence, Florence, Italy.
EM massimo.bongi@fi.infn.it
NR 11
TC 0
Z9 0
U1 1
U2 1
PU ELSEVIER SCIENCE BV
PI AMSTERDAM
PA PO BOX 211, 1000 AE AMSTERDAM, NETHERLANDS
SN 2405-6014
EI 1873-3832
J9 NUCL PART PHYS P
JI Nucl. Part. Phys. Proc.
PD OCT-DEC
PY 2016
VL 279
BP 125
EP 129
DI 10.1016/j.nuclphysbps.2016.10.018
PG 5
GA ED8FJ
UT WOS:000389107100018
ER
PT J
AU Zhou, ZG
Wong, J
Mahin, S
AF Zhou, Zhiguang
Wong, Jenna
Mahin, Stephen
TI Potentiality of Using Vertical and Three-Dimensional Isolation Systems
in Nuclear Structures
SO NUCLEAR ENGINEERING AND TECHNOLOGY
LA English
DT Article
DE 3D Isolation Systems; Isolator; Nuclear Power Plant; Response Spectrum;
Rocking Effect; Vertical Isolation
AB Although the horizontal component of an earthquake response can be significantly reduced through the use of conventional seismic isolators, the vertical component of excitation is still transmitted directly into the structure. Records from instrumented structures, and some recent tests and analyses have actually seen increases in vertical responses in base isolated structures under the combined effects of horizontal and vertical ground motions. This issue becomes a great concern to facilities such as a Nuclear Power Plants (NPP), with specialized equipment and machinery that is not only expensive, but critical to safe operation. As such, there is considerable interest worldwide in vertical and three-dimensional (3D) isolation systems. This paper examines several vertical and 3D isolation systems that have been proposed and their potential application to modern nuclear facilities. In particular, a series of case study analyses of a modern NPP model are performed to examine the benefits and challenges associated with 3D isolation compared with horizontal isolation. It was found that compared with the general horizontal isolators, isolators that have vertical frequencies of no more than 3 Hz can effectively reduce the vertical in-structure responses for the studied NPP model. Among the studied cases, the case that has a vertical isolation frequency of 3 Hz is the one that can keep the horizontal period of the isolators as the first period while having the most flexible vertical isolator properties. When the vertical frequency of isolators reduces to 1 Hz, the rocking effect is obvious and rocking restraining devices are necessary. Copyright (C) 2016, Published by Elsevier Korea LLC on behalf of Korean Nuclear Society.
C1 [Zhou, Zhiguang] Tongji Univ, Res Inst Struct Engn & Disaster Reduct, 1239 Siping Rd, Shanghai 200092, Peoples R China.
[Wong, Jenna] Lawrence Berkeley Natl Labs, 1 Cyclotron Rd,MS74R316C, Berkeley, CA 94720 USA.
[Mahin, Stephen] Univ Calif Berkeley, Dept Civil & Environm Engn, 777 Davis Hall, Berkeley, CA 94720 USA.
RP Zhou, ZG (reprint author), Tongji Univ, Res Inst Struct Engn & Disaster Reduct, 1239 Siping Rd, Shanghai 200092, Peoples R China.
EM zgzhou@tongji.edu.cn
FU National Natural Science Foundation of China [51478357, 51308418];
National Science and Technology Pillar Program [2015BAK17B04]; KEPCO
Engineering and Construction Company Inc.; Electric Power Research
Institute
FX The authors wish to gratefully acknowledge the support for this work by
the National Natural Science Foundation of China under Grant Numbers
51478357 and 51308418, National Science and Technology Pillar Program
Number 2015BAK17B04, a cooperative research program funded by KEPCO
Engineering and Construction Company Inc., and a research program funded
by the Electric Power Research Institute.
NR 23
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U1 3
U2 3
PU KOREAN NUCLEAR SOC
PI DAEJEON
PA NUTOPIA BLDG, 342-1 JANGDAE-DONG, DAEJEON, 305-308, SOUTH KOREA
SN 1738-5733
J9 NUCL ENG TECHNOL
JI Nucl. Eng. Technol.
PD OCT
PY 2016
VL 48
IS 5
BP 1237
EP 1251
DI 10.1016/j.net.2016.03.005
PG 15
WC Nuclear Science & Technology
SC Nuclear Science & Technology
GA EA6MQ
UT WOS:000386743700017
ER
PT J
AU Knapik, JJ
Jean, RT
Austin, KG
Steelman, RA
Gannon, J
Farina, EK
Lieberman, HR
AF Knapik, Joseph J.
Jean, Rosenie T.
Austin, Krista G.
Steelman, Ryan A.
Gannon, Julia
Farina, Emily K.
Lieberman, Harris R.
TI Temporal trends in dietary supplement prescriptions of United States
military service members suggest a decrease in pyridoxine and increase
in vitamin D supplements from 2005 to 2013
SO NUTRITION RESEARCH
LA English
DT Article
DE Multivitamins; Vitamins; Minerals; Antacids/absorbents; Iron
preparations; Cathartics/laxatives
ID NUTRITION EXAMINATION SURVEY; CARPAL-TUNNEL-SYNDROME; RANDOMIZED
CONTROLLED-TRIAL; HEART-DISEASE INCIDENCE; CARDIOVASCULAR-DISEASE;
COMMON-COLD; PRIMARY PREVENTION; C SUPPLEMENTATION; NATIONAL-HEALTH;
CLINICAL-TRIAL
AB Dietary supplements (DSs) can be obtained over-the-counter but can also be prescribed by health-care providers for therapeutic reasons. Few studies have documented this later source despite the fact that 79% of physicians and 82% of nurses have recommended DSs to patients. This investigation assessed prevalence and temporal trends in oral DS prescriptions filled by all United States service members (SMs) from 2005 to 2013 (n = 1 427 080 +/- 22 139, mean +/- standard deviation (SD)/y). We hypothesize that there would be temporal variations in specific types of DSs. Data obtained from Department of Defense Pharmacy Data Transaction System were grouped by American Hospital Formulary System pharmacologic-therapeutic classifications and prevalence examined over time. About 11% of SMs filled one or more DS prescriptions of 235 180 +/- 4926 (mean +/- SD) prescriptions/y over the 9 -year period. Curve -fitting techniques indicated significant linear declines over time for multivitamins (P = .004), iron preparations (P < .001), antacids (P < .001), and vitamin B and B complex vitamins (P < .001). There were significant quadratic trends indicating a rise in early years followed by a leveling off in later years for replacement preparations (P < .001) and vitamin C (P < .001). There were significant quadratic trends (P < .001) for vitamin E indicating a decline in early years and leveling off in later years, and vitamin D indicating little change in early years followed by a large rise subsequently (P < .001). This study identified temporal trends in specific DS categories that may be associated with changing perceptions of prescribers and/or patients of the appropriate roles of DSs in medicine and public health. Published by Elsevier Inc.
C1 [Knapik, Joseph J.; Austin, Krista G.; Farina, Emily K.; Lieberman, Harris R.] US Army, Environm Med Res Inst, 10 Gen Greene Ave USARIEM, Natick, MA 01760 USA.
[Knapik, Joseph J.; Steelman, Ryan A.] US Army, Publ Hlth Ctr, Aberdeen Proving Ground, MD 21010 USA.
[Knapik, Joseph J.; Austin, Krista G.; Farina, Emily K.] Oak Ridge Inst Sci & Educ, Belcamp, MD 21017 USA.
[Jean, Rosenie T.; Gannon, Julia] US Army, Surg Gen, Pharmacovigilance Ctr, Falls Church, VA 22041 USA.
RP Knapik, JJ (reprint author), US Army, Environm Med Res Inst, 10 Gen Greene Ave USARIEM, Natick, MA 01760 USA.; Knapik, JJ (reprint author), US Army, Publ Hlth Ctr, Aberdeen Proving Ground, MD 21010 USA.; Knapik, JJ (reprint author), Oak Ridge Inst Sci & Educ, Belcamp, MD 21017 USA.
EM joseph.j.knapik.ctr@mail.mil; rosenie.thelus.civ@mail.mil;
krista.g.austin.ctr@mail.mil; ryan.a.steelman.ctr@mail.mil;
julia.f.gannon.civ@mail.mil; emily.k.farina.ctr@mail.mil;
harris.r.lieberman.civ@mail.mil
OI Knapik, Joseph/0000-0002-1568-1860
FU US Army Research Institute of Environmental Medicine (USARIEM); Army
Institute of Public Health; Center Alliance for Nutrition and Dietary
Supplement Research
FX Thanks to Angie Cost from the Armed Forces Health Surveillance Branch of
the Defense Health Agency for providing denominators that allowed
calculation of prevalences. This research was supported in part by an
appointment to the Knowledge Preservation Program at the US Army
Research Institute of Environmental Medicine (USARIEM) and the Army
Institute of Public Health administered by the Oak Ridge Institute for
Science and Education through an interagency agreement between the US
Department of Energy and USARIEM. Funding was also provided by the
Center Alliance for Nutrition and Dietary Supplement Research. No author
has a conflict of interest.
NR 109
TC 1
Z9 1
U1 9
U2 9
PU PERGAMON-ELSEVIER SCIENCE LTD
PI OXFORD
PA THE BOULEVARD, LANGFORD LANE, KIDLINGTON, OXFORD OX5 1GB, ENGLAND
SN 0271-5317
J9 NUTR RES
JI Nutr. Res.
PD OCT
PY 2016
VL 36
IS 10
BP 1140
EP 1152
DI 10.1016/j.nutres.2016.09.001
PG 13
WC Nutrition & Dietetics
SC Nutrition & Dietetics
GA EE0SG
UT WOS:000389288600011
PM 27865356
ER
PT J
AU Reilly, AC
Staid, A
Gao, M
Guikema, SD
AF Reilly, Allison C.
Staid, Andrea
Gao, Michael
Guikema, Seth D.
TI Tutorial: Parallel Computing of Simulation Models for Risk Analysis
SO RISK ANALYSIS
LA English
DT Article
DE Parallel computing; risk analysis
ID MONTE-CARLO-SIMULATION; UNCERTAINTY
AB Simulation models are widely used in risk analysis to study the effects of uncertainties on outcomes of interest in complex problems. Often, these models are computationally complex and time consuming to run. This latter point may be at odds with time-sensitive evaluations or may limit the number of parameters that are considered. In this article, we give an introductory tutorial focused on parallelizing simulation code to better leverage modern computing hardware, enabling risk analysts to better utilize simulation-based methods for quantifying uncertainty in practice. This article is aimed primarily at risk analysts who use simulation methods but do not yet utilize parallelization to decrease the computational burden of these models. The discussion is focused on conceptual aspects of embarrassingly parallel computer code and software considerations. Two complementary examples are shown using the languages MATLAB and R. A brief discussion of hardware considerations is located in the Appendix.
C1 [Reilly, Allison C.; Guikema, Seth D.] Univ Michigan, Ind & Operat Res, 1205 Beal Ave, Ann Arbor, MI 48109 USA.
[Staid, Andrea] Sandia Natl Labs, Discrete Math & Optimizat, POB 5800, Albuquerque, NM 87185 USA.
[Gao, Michael] SolarCity, San Mateo, CA USA.
RP Reilly, AC (reprint author), Univ Michigan, Ind & Operat Res, 1205 Beal Ave, Ann Arbor, MI 48109 USA.
EM acreilly@umich.edu
FU National Science Foundation (NSF) [1243482, 1149460]
FX This work is funded by from the National Science Foundation (NSF),
grants 1243482 and 1149460. The support of the sponsor is gratefully
acknowledged. Any opinions, findings, conclusions, or recommendations
presented in this article are those of the authors and do not
necessarily reflect the view of the National Science Foundation.
NR 16
TC 0
Z9 0
U1 3
U2 3
PU WILEY-BLACKWELL
PI HOBOKEN
PA 111 RIVER ST, HOBOKEN 07030-5774, NJ USA
SN 0272-4332
EI 1539-6924
J9 RISK ANAL
JI Risk Anal.
PD OCT
PY 2016
VL 36
IS 10
BP 1844
EP 1854
DI 10.1111/risa.12565
PG 11
WC Public, Environmental & Occupational Health; Mathematics,
Interdisciplinary Applications; Social Sciences, Mathematical Methods
SC Public, Environmental & Occupational Health; Mathematics; Mathematical
Methods In Social Sciences
GA ED6RZ
UT WOS:000388984900003
PM 26849834
ER
PT J
AU Kuhlgert, S
Austic, G
Zegarac, R
Osei-Bonsu, I
Hoh, D
Chilvers, MI
Roth, MG
Bi, K
TerAvest, D
Weebadde, P
Kramer, DM
AF Kuhlgert, Sebastian
Austic, Greg
Zegarac, Robert
Osei-Bonsu, Isaac
Hoh, Donghee
Chilvers, Martin I.
Roth, Mitchell G.
Bi, Kevin
TerAvest, Dan
Weebadde, Prabode
Kramer, David M.
TI MultispeQ Beta: a tool for large-scale plant phenotyping connected to
the open PhotosynQ network
SO Royal Society Open Science
LA English
DT Article
DE agriculture; chlorophyll fluorescence; open-source hardware; phenomics;
photosynthesis
ID SUDDEN-DEATH SYNDROME; CYCLIC ELECTRON FLOW; CHLOROPHYLL FLUORESCENCE;
ABSORBENCY CHANGES; CITIZEN SCIENCE; ATP SYNTHASE; IN-VIVO; LIGHT;
STATE; ABSORPTION
AB Large-scale high-throughput plant phenotyping (sometimes called phenomics) is becoming increasingly important in plant biology and agriculture and is essential to cutting-edge plant breeding and management approaches needed to meet the food and fuel needs for the next century. Currently, the application of these approaches is severely limited by the availability of appropriate instrumentation and by the ability to communicate experimental protocols, results and analyses. To address these issues, we have developed a low-cost, yet sophisticated open-source scientific instrument designed to enable communities of researchers, plant breeders, educators, farmers and citizen scientists to collect high-quality field data on a large scale. The MultispeQ provides measurements in the field or laboratory of both, environmental conditions (light intensity and quality, temperature, humidity, CO2 levels, time and location) and useful plant phenotypes, including photosynthetic parameters-photosystem II quantum yield (FII), non-photochemical exciton quenching (NPQ), photosystem II photoinhibition, light-driven proton translocation and thylakoid proton motive force, regulation of the chloroplast ATP synthase and potentially many others-and leaf chlorophyll and other pigments. Plant phenotype data are transmitted from the MultispeQ to mobile devices, laptops or desktop computers together with key metadata that gets saved to the PhotosynQ platform (https://photosynq.org) and provides a suite of web-based tools for sharing, visualization, filtering, dissemination and analyses. We present validation experiments, comparing MultispeQ results with established platforms, and show that it can be usefully deployed in both laboratory and field settings. We present evidence that MultispeQ can be used by communities of researchers to rapidly measure, store and analyse multiple environmental and plant properties, allowing for deeper understanding of the complex interactions between plants and their environment.
C1 [Kuhlgert, Sebastian; Austic, Greg; Zegarac, Robert; Osei-Bonsu, Isaac; Hoh, Donghee; Bi, Kevin; TerAvest, Dan; Kramer, David M.] Michigan State Univ, MSU DOE Plant Res Lab, E Lansing, MI 48824 USA.
[Chilvers, Martin I.; Roth, Mitchell G.] Michigan State Univ, Dept Plant Soil & Microbial Sci, E Lansing, MI 48824 USA.
[Chilvers, Martin I.; Roth, Mitchell G.] Michigan State Univ, Grad Program Genet, E Lansing, MI 48824 USA.
[Weebadde, Prabode] Venturit Inc, E Lansing, MI USA.
RP Kramer, DM (reprint author), Michigan State Univ, MSU DOE Plant Res Lab, E Lansing, MI 48824 USA.
EM kramerd8@cns.msu.edu
OI Osei-Bonsu, Isaac/0000-0002-4764-1951
FU U.S. Department of Energy (DOE), Office of Science, Basic Energy
Sciences (BES) [DE-FG02-91ER20021]; MSU AgBioResearch program; USAID;
McKnight Foundation
FX The development and testing of the MultispeQ device and PhotosynQ
platform (contributions from S.K., G.A., D.T. and D.M.K.) were supported
by the U.S. Department of Energy (DOE), Office of Science, Basic Energy
Sciences (BES) under Award no. DE-FG02-91ER20021 with foundational
support from the MSU Center for Advanced Algal and Plant Phenotyping
(CAAPP) and the MSU AgBioResearch program. The fieldwork (I.O.-B. and
D.H.) was supported by the US Agency for International development
(USAID, through the Legume Innovation Lab). The applications of the
platform for plant stress analysis, funding D.T. and G.A., were
supported by grants from USAID and the McKnight Foundation.
NR 57
TC 0
Z9 0
U1 10
U2 10
PU ROYAL SOC
PI LONDON
PA 6-9 CARLTON HOUSE TERRACE, LONDON SW1Y 5AG, ENGLAND
SN 2054-5703
J9 ROY SOC OPEN SCI
JI R. Soc. Open Sci.
PD OCT
PY 2016
VL 3
IS 10
AR 160592
DI 10.1098/rsos.160592
PG 17
WC Multidisciplinary Sciences
SC Science & Technology - Other Topics
GA EE0CS
UT WOS:000389241700051
ER
PT J
AU Wood, E
Duran, A
Kelly, K
AF Wood, Eric
Duran, Adam
Kelly, Kenneth
TI EPA GHG Certification of Medium- and Heavy-Duty Vehicles: Development of
Road Grade Profiles Representative of US Controlled Access Highways
SO SAE International Journal of Commercial Vehicles
LA English
DT Article
AB In collaboration with the U.S. Environmental Protection Agency and the U.S. Department of Energy, the National Renewable Energy Laboratory has conducted a national analysis of road grade characteristics experienced by U.S. medium-and heavy-duty trucks on controlled access highways. These characteristics have been developed using TomTom's commercially available street map and road grade database. Using the TomTom national road grade database, national statistics on road grade and hill distances were generated for the U.S. network of controlled access highways. These statistical distributions were then weighted using data provided by the U.S. Environmental Protection Agency for activity of medium-and heavy-duty trucks on controlled access highways. The national activity-weighted road grade and hill distance distributions were then used as targets for development of a handful of sample grade profiles potentially to be used in the U.S. Environmental Protection Agency's Greenhouse Gas Emissions Model certification tool as well as in dynamometer testing of medium-and heavy-duty vehicles and their powertrains.
C1 [Wood, Eric; Duran, Adam; Kelly, Kenneth] Natl Renewable Energy Lab, Golden, CO USA.
RP Wood, E; Duran, A; Kelly, K (reprint author), Natl Renewable Energy Lab, Transportat & Hydrogen Syst Ctr, 15013 Denver West Pkwy MS 1634, Golden, CO 80401 USA.
EM eric.wood@nrel.gov; adam.duran@nrel.gov; kenneth.kelly@nrel.gov
NR 15
TC 0
Z9 0
U1 0
U2 0
PU SAE INT
PI WARRENDALE
PA 400 COMMONWEALTH DR, WARRENDALE, PA 15096 USA
SN 1946-391X
EI 1946-3928
J9 SAE INT J COMMER VEH
JI SAE Int. J. Commer. Veh.
PD OCT
PY 2016
VL 9
IS 2
BP 94
EP 104
DI 10.4271/2016-01-8017
PG 11
WC Transportation Science & Technology
SC Transportation
GA ED9ZX
UT WOS:000389233800007
ER
PT J
AU Prohaska, R
Konan, A
Kelly, K
Lammert, M
AF Prohaska, Robert
Konan, Arnaud
Kelly, Kenneth
Lammert, Michael
TI Heavy-Duty Vehicle Port Drayage Drive Cycle Characterization and
Development
SO SAE International Journal of Commercial Vehicles
LA English
DT Article
AB In an effort to better understand the operational requirements of port drayage vehicles and their potential for adoption of advanced technologies, National Renewable Energy Laboratory (NREL) researchers collected over 36,000 miles of in-use duty cycle data from 30 Class 8 drayage trucks operating at the Port of Long Beach and Port of Los Angeles in Southern California. These data include 1-Hz global positioning system location and SAE J1939 high-speed controller area network information. Researchers processed the data through NREL's Drive-Cycle Rapid Investigation, Visualization, and Evaluation tool to examine vehicle kinematic and dynamic patterns across the spectrum of operations. Using the k-medoids clustering method, a repeatable and quantitative process for multi-mode drive cycle segmentation, the analysis led to the creation of multiple drive cycles representing four distinct modes of operation that can be used independently or in combination. These drive cycles are statistically representative of real-world operation of port drayage vehicles. When combined with modeling and simulation tools, these representative test cycles allow advanced vehicle or systems developers to efficiently and accurately evaluate vehicle technology performance requirements to reduce cost and development time while ultimately leading to the commercialization of advanced technologies that meet the performance requirements of the port drayage vocation. The drive cycles, which are suitable for chassis dynamometer testing, were compared to several existing test cycles. This paper presents the clustering methodology, accompanying results of the port drayage duty cycle analysis and custom drive cycle creation.
C1 [Prohaska, Robert] Natl Renewable Energy Lab, Simulat Testing & Integrat Grp, Medium & Heavy Duty Fleet Test & Evaluat Projects, Golden, CO 80401 USA.
[Konan, Arnaud; Lammert, Michael] Natl Renewable Energy Lab, Transportat & Hydrogen Syst Ctr, Golden, CO USA.
[Kelly, Kenneth] Natl Renewable Energy Lab, Golden, CO USA.
RP Prohaska, R (reprint author), Natl Renewable Energy Lab, Simulat Testing & Integrat Grp, Medium & Heavy Duty Fleet Test & Evaluat Projects, Golden, CO 80401 USA.
EM Robert.Prohaska@nrel.gov; Arnaud.Konan@nrel.gov; Kenneth.Kelly@nrel.gov;
Michael.Lammert@nrel.gov
NR 17
TC 0
Z9 0
U1 0
U2 0
PU SAE INT
PI WARRENDALE
PA 400 COMMONWEALTH DR, WARRENDALE, PA 15096 USA
SN 1946-391X
EI 1946-3928
J9 SAE INT J COMMER VEH
JI SAE Int. J. Commer. Veh.
PD OCT
PY 2016
VL 9
IS 2
BP 331
EP 338
DI 10.4271/2016-01-8135
PG 8
WC Transportation Science & Technology
SC Transportation
GA ED9ZX
UT WOS:000389233800023
ER
PT J
AU Watkins, EB
Majewski, J
Baldwin, JK
Chen, Y
Li, N
Hoagland, RG
Yadav, SK
Liu, XY
Beyerlein, IJ
Mara, NA
AF Watkins, E. B.
Majewski, J.
Baldwin, J. K.
Chen, Y.
Li, N.
Hoagland, R. G.
Yadav, S. K.
Liu, X. -Y.
Beyerlein, I. J.
Mara, N. A.
TI Neutron reflectometry investigations of interfacial structures of Ti/TiN
layers deposited by magnetron sputtering
SO THIN SOLID FILMS
LA English
DT Article
DE Titanium; Titanium nitride; Engineered interfaces; Composite materials;
Neutron reflectivity
ID TRANSMISSION ELECTRON-MICROSCOPY; IN-SITU NANOINDENTATION; NANOLAYERED
COMPOSITES; MECHANICAL-PROPERTIES; MULTILAYER COATINGS; DIFFUSION
BARRIER; TIN; BEHAVIOR; THICKNESS; HARDNESS
AB Nanolayered metal-ceramic composite systems provide the possibility to produce new materials with exceptional strength, toughness, and radiation resistance not exhibited by their individual constituents. The unusual behaviors are frequently attributed to the high density of internal interfaces. Most layered structures studied to date contain sharp interfaces and the synthesis of more diffuse interfacial structures, where the interface is graded out of the interface plane, has not been deeply explored. Here we show how neutron reflectometry was used to study the structure of magnetron sputter deposited titanium and titanium nitride (Ti/fiN) layers as a function of deposition parameters: temperature, rate of N-2 flow or pressure, electrical bias applied to the sample, and orientation of the ion source relative to the sample. These different deposition and post-processing strategies resulted in profound changes in the structure of the interfacial region between the two components in Ti/TiNx bilayers. The results show that temperature and low step-wise N-2 flow rates, but not electrical bias, can form graded interfaces in a controlled manner. (C) 2016 Elsevier B.V. All rights reserved.
C1 [Watkins, E. B.] Los Alamos Natl Lab, Mat Phys & Applicat Div, MPA 11, Los Alamos, NM 87545 USA.
[Majewski, J.; Baldwin, J. K.; Chen, Y.; Li, N.; Mara, N. A.] Los Alamos Natl Lab, Ctr Integrated Nanotechnol, Mat Phys & Applicat Div, Los Alamos, NM 87545 USA.
[Majewski, J.] Univ Calif Davis, Dept Chem Engn, Davis, CA 95616 USA.
[Hoagland, R. G.; Yadav, S. K.; Liu, X. -Y.] Los Alamos Natl Lab, Mat Sci & Technol Div, MST 8, Los Alamos, NM 87545 USA.
[Beyerlein, I. J.] Los Alamos Natl Lab, Div Theoret, Fluid Dynam & Solid Mech, T-3, Los Alamos, NM 87545 USA.
[Mara, N. A.] Los Alamos Natl Lab, Inst Mat Sci, Los Alamos, NM 87545 USA.
RP Majewski, J (reprint author), Los Alamos Natl Lab, Ctr Integrated Nanotechnol, Mat Phys & Applicat Div, Los Alamos, NM 87545 USA.
EM jarek@lanl.gov
RI Li, Nan /F-8459-2010; Chen, Youxing/P-5006-2016; Yadav,
Satyesh/M-6588-2014
OI Li, Nan /0000-0002-8248-9027; Chen, Youxing/0000-0003-1111-4495;
FU U.S. Department of Energy, Office of Science, Office of Basic Energy
Sciences; U.S. Department of Energy [DE-AC52-06NA25396]
FX The authors gratefully acknowledge support from the U.S. Department of
Energy, Office of Science, Office of Basic Energy Sciences. This work
was performed, in part, at the Center for Integrated Nanotechnologies,
an Office of Science User Facility operated for the U.S. Department of
Energy (DOE) Office of Science. Los Alamos National Laboratory, an
affirmative action equal opportunity employer, is operated by Los Alamos
National Security, LLC, for the National Nuclear Security Administration
of the U.S. Department of Energy under Contract DE-AC52-06NA25396. This
work also benefited from the use of the Lujan Neutron Scattering Center
at LANSCE.
NR 51
TC 0
Z9 0
U1 4
U2 4
PU ELSEVIER SCIENCE SA
PI LAUSANNE
PA PO BOX 564, 1001 LAUSANNE, SWITZERLAND
SN 0040-6090
J9 THIN SOLID FILMS
JI Thin Solid Films
PD OCT 1
PY 2016
VL 616
BP 399
EP 407
DI 10.1016/j.tsf.2016.08.064
PG 9
WC Materials Science, Multidisciplinary; Materials Science, Coatings &
Films; Physics, Applied; Physics, Condensed Matter
SC Materials Science; Physics
GA EE2BL
UT WOS:000389388600057
ER
PT J
AU Maffia, GJ
Gaffney, AM
Mason, OM
AF Maffia, Gennaro J.
Gaffney, Anne M.
Mason, Olivia M.
TI Techno-Economic Analysis of Oxidative Dehydrogenation Options
SO TOPICS IN CATALYSIS
LA English
DT Article; Proceedings Paper
CT 7th Irsee Symposium on New Insights in Selective Oxidation Catalysis,
Electrocatalysis, and Catalysis of Biomass
CY JUN 04-07, 2015
CL Irsee, GERMANY
SP Robert Karl Grasselli Fdn
DE Pyrolysis; Oxidative dehydrogenation; Shutdown economics; Stoichiometric
selectivities
AB The world-wide market for light olefins will approach one trillion pounds per year by the year 2020. Light olefins are conventionally produced by the steam cracking of hydrocarbons from ethane to gas oil. This technology is decades old and results in a wide range of by-products, some valuable, some with fuel value, and some requiring waste treatment before disposal. An economic analysis was performed using a cost of production procedure commonly called a required netback analysis. These results were compared with the expected performance of a novel catalytic route with very high selectivity, running at much lower temperatures and similar pressures. The new route uses a mixed metal oxide catalyst in packed tubes with a heat transfer fluid in the reactor shell for heat management. Results indicate that the new route has much lower variable cost, fixed costs and capital recovery reaching shutdown economic level.
C1 [Maffia, Gennaro J.] Manhattan Coll, Dept Chem Engn, Riverdale, NY USA.
[Gaffney, Anne M.; Mason, Olivia M.] Idaho Natl Lab, POB 1625m MS 2203, Idaho Falls, ID 83415 USA.
RP Maffia, GJ (reprint author), Manhattan Coll, Dept Chem Engn, Riverdale, NY USA.
EM gennaro.maffia@manhattan.edu
NR 6
TC 0
Z9 0
U1 4
U2 4
PU SPRINGER/PLENUM PUBLISHERS
PI NEW YORK
PA 233 SPRING ST, NEW YORK, NY 10013 USA
SN 1022-5528
EI 1572-9028
J9 TOP CATAL
JI Top. Catal.
PD OCT
PY 2016
VL 59
IS 17-18
BP 1573
EP 1579
DI 10.1007/s11244-016-0677-9
PG 7
WC Chemistry, Applied; Chemistry, Physical
SC Chemistry
GA ED4NE
UT WOS:000388825200012
ER
PT J
AU Sevanto, S
Xu, CG
AF Sevanto, Sanna
Xu, Chonggang
TI Towards more accurate vegetation mortality predictions
SO TREE PHYSIOLOGY
LA English
DT Article
ID INDUCED TREE MORTALITY; LODGEPOLE PINE TREES; CARBON ALLOCATION;
WOODY-PLANTS; GROWTH; DROUGHT; VIGOR; MECHANISMS; EUCALYPTUS; DYNAMICS
C1 [Sevanto, Sanna; Xu, Chonggang] Los Alamos Natl Lab, Earth & Environm Sci Div, POB 1663,MS J535, Los Alamos, NM 87545 USA.
RP Sevanto, S (reprint author), Los Alamos Natl Lab, Earth & Environm Sci Div, POB 1663,MS J535, Los Alamos, NM 87545 USA.
EM sanna@lanl.gov
OI Xu, Chonggang/0000-0002-0937-5744
FU Los Alamos National Laboratory Directors Research and Development
program [20150030ER]
FX This piece of work was supported by Los Alamos National Laboratory
Directors Research and Development program project #20150030ER.
NR 36
TC 0
Z9 0
U1 6
U2 6
PU OXFORD UNIV PRESS
PI OXFORD
PA GREAT CLARENDON ST, OXFORD OX2 6DP, ENGLAND
SN 0829-318X
EI 1758-4469
J9 TREE PHYSIOL
JI Tree Physiol.
PD OCT
PY 2016
VL 36
IS 10
BP 1191
EP 1195
DI 10.1093/treephys/tpw082
PG 5
WC Forestry
SC Forestry
GA ED6CK
UT WOS:000388942100001
PM 27672190
ER
PT J
AU Qin, Y
Sammond, DW
Braselmann, E
Carpenter, MC
Palmer, AE
AF Qin, Yan
Sammond, Deanne W.
Braselmann, Esther
Carpenter, Margaret C.
Palmer, Amy E.
TI Development of an Optical Zn2+ Probe Based on a Single Fluorescent
Protein
SO ACS CHEMICAL BIOLOGY
LA English
DT Article
ID GCAMP CALCIUM INDICATOR; NEURAL ACTIVITY; METAL-IONS; SENSORS; FRET;
ZINC; MITOCHONDRIAL; REVEAL; CELLS
AB Various fluorescent probes have been developed to reveal the biological functions of intracellular labile Zn2+. Here, we present Green Zinc Probe (GZnP), a novel genetically encoded Zn2+ sensor design based on a single fluorescent protein (single-FP). The GZnP sensor is generated by attaching two zinc fingers (ZF) of the transcription factor Zap1 (ZF1 and ZF2) to the two ends of a circularly permuted green fluorescent protein (cpGFP). Formation of ZF folds induces interaction between the two ZFs, which induces a change in the cpGFP conformation, leading to an increase in fluorescence. A small sensor library is created to include mutations in the ZFs, cpGFP and linkers between ZF and cpGFP to improve signal stability, sensor brightness and dynamic range based on rational protein engineering, and computational design by Rosetta. Using a cell-based library screen, we identify sensor GZnP1, which demonstrates a stable maximum signal, decent brightness (QY = 0.42 at apo state), as well as specific and sensitive response to Zn2+ in HeLa cells (F-max/F-min = 2.6, K-d = 58 pM, pH 7.4). The subcellular localizing sensors mito-GZnP1 (in mitochondria matrix) and Lck-GZnP1 (on plasma membrane) display sensitivity to Zn2+ (F-max/F-min = 2.2). This sensor design provides freedom to be used in combination with other optical indicators and optogenetic tools for simultaneous imaging and advancing our understanding of cellular Zn2+ function.
C1 [Qin, Yan; Braselmann, Esther; Carpenter, Margaret C.; Palmer, Amy E.] Univ Colorado, Dept Chem & Biochem, Boulder, CO 80303 USA.
[Qin, Yan; Braselmann, Esther; Carpenter, Margaret C.; Palmer, Amy E.] Univ Colorado, BioFrontiers Inst, Boulder, CO 80303 USA.
[Sammond, Deanne W.] Natl Renewable Energy Lab, Biosci Ctr, Golden, CO 80401 USA.
[Qin, Yan] Univ Denver, Dept Biol Sci, Denver, CO 80208 USA.
RP Qin, Y; Palmer, AE (reprint author), Univ Colorado, Dept Chem & Biochem, Boulder, CO 80303 USA.; Qin, Y; Palmer, AE (reprint author), Univ Colorado, BioFrontiers Inst, Boulder, CO 80303 USA.; Qin, Y (reprint author), Univ Denver, Dept Biol Sci, Denver, CO 80208 USA.
EM Yan.Qin@du.edu; Amy.Palmer@colorado.edu
FU NIH [R01 GM084027]; NIST-CU [70NANB15H226]; U.S. Department of Energy's
Bioenergy Technologies Office (DOE-BETO) [DE-AC36-08GO28308]; National
Renewable Energy Laboratory; [K99/R00 EB017289]
FX We would like to acknowledge the following sources for general financial
support: K99/R00 EB017289 (to Y.Q.) and NIH R01 GM084027 (to A.E.P.).
The Nikon A1R microscope was acquired through the generous support of
NIST-CU Cooperative Agreement award number 70NANB15H226. This work was
funded by the U.S. Department of Energy's Bioenergy Technologies Office
(DOE-BETO), Contract No. DE-AC36-08GO28308 with the National Renewable
Energy Laboratory. The authors declare no conflict of interest.
NR 28
TC 0
Z9 1
U1 6
U2 6
PU AMER CHEMICAL SOC
PI WASHINGTON
PA 1155 16TH ST, NW, WASHINGTON, DC 20036 USA
SN 1554-8929
EI 1554-8937
J9 ACS CHEM BIOL
JI ACS Chem. Biol.
PD OCT
PY 2016
VL 11
IS 10
BP 2744
EP 2751
DI 10.1021/acschembio.6b00442
PG 8
WC Biochemistry & Molecular Biology
SC Biochemistry & Molecular Biology
GA DZ9IE
UT WOS:000386187700010
PM 27467056
ER
PT J
AU He, LY
AF He, Lianyi
TI Dynamic density and spin responses of a superfluid Fermi gas in the
BCS-BEC crossover: Path integral formulation and pair fluctuation theory
SO ANNALS OF PHYSICS
LA English
DT Article
DE BCS-BEC crossover; Density response; Spin response
ID EQUATION-OF-STATE; BOSE-CONDENSATION; UNIVERSAL THERMODYNAMICS; QUARK
MATTER; SUPERCONDUCTIVITY; PSEUDOGAP; EVOLUTION
AB We present a standard field theoretical derivation of the dynamic density and spin linear response functions of a dilute superfluid Fermi gas in the BCS-BEC crossover in both three and two dimensions. The derivation of the response functions is based on the elegant functional path integral approach which allows us to calculate the density-density and spin-spin correlation functions by introducing the external sources for the density and the spin density. Since the generating functional cannot be evaluated exactly, we consider two gapless approximations which ensure a gap less collective mode (Goldstone mode) in the superfluid state: the BCS-Leggett mean-field theory and the Gaussian-pair-fluctuation (GPF) theory. In the mean-field theory, our results of the response functions agree with the known results from the random phase approximation. We further consider the pair fluctuation effects and establish a theoretical framework for the dynamic responses within the GPF theory. We show that the GPF response theory naturally recovers three kinds of famous diagrammatic contributions: the Self-Energy contribution, the Aslamazov-Lakin contribution, and the Maki-Thompson contribution. We also show that unlike the equilibrium state, in evaluating the response functions, the linear (first-order) terms in the external sources as well as the induced order parameter perturbations should be treated carefully. In the superfluid state, there is an additional order parameter contribution which ensures that in the static and long wavelength limit, the density response function recovers the result of the compressibility (compressibility sum rule). We expect that the f-sum rule is manifested by the full number equation which includes the contribution from the Gaussian pair fluctuations. The dynamic density and spin response functions in the normal phase (above the superfluid critical temperature) are also derived within the Nozieres-Schmitt-Rink (NSR) theory. (C) 2016 Elsevier Inc. All rights reserved.
C1 [He, Lianyi] Los Alamos Natl Lab, Div Theoret, Los Alamos, NM 87545 USA.
[He, Lianyi] Tsinghua Univ, Dept Phys, Beijing 100084, Peoples R China.
[He, Lianyi] Tsinghua Univ, Collaborat Innovat Ctr Quantum Matter, Beijing 100084, Peoples R China.
RP He, LY (reprint author), Tsinghua Univ, Dept Phys, Beijing 100084, Peoples R China.
EM lianyi@mail.tsinghua.edu.cn
RI He, Lianyi/G-5110-2010
OI He, Lianyi/0000-0002-9965-0446
FU US Department of Energy Nuclear Physics Office [DE-AC02-05CH11231]; Los
Alamos National Laboratory, Tsinghua University; Thousand Young Talent
Program in China
FX The author thanks Joseph Carlson and Stefano Gandolfi for guiding him to
the topic of the dynamic density and spin density responses. He also
thanks Hui Hu for useful discussions. The Feynman diagrams were plotted
by Yin Jiang. The work is supported by the US Department of Energy
Nuclear Physics Office (No. DE-AC02-05CH11231), Los Alamos National
Laboratory, Tsinghua University, and Thousand Young Talent Program in
China.
NR 101
TC 3
Z9 3
U1 1
U2 1
PU ACADEMIC PRESS INC ELSEVIER SCIENCE
PI SAN DIEGO
PA 525 B ST, STE 1900, SAN DIEGO, CA 92101-4495 USA
SN 0003-4916
EI 1096-035X
J9 ANN PHYS-NEW YORK
JI Ann. Phys.
PD OCT
PY 2016
VL 373
BP 470
EP 511
DI 10.1016/j.aop.2016.07.030
PG 42
WC Physics, Multidisciplinary
SC Physics
GA EB9RJ
UT WOS:000387734500032
ER
PT J
AU Pasyanos, ME
Gok, R
Walter, WR
AF Pasyanos, Michael E.
Gok, Rengin
Walter, William R.
TI 2D Variations in Coda Amplitudes in the Middle East
SO BULLETIN OF THE SEISMOLOGICAL SOCIETY OF AMERICA
LA English
DT Article
ID WAVE ATTENUATION; TOMOGRAPHY
AB Coda amplitudes have proven to be a stable feature of seismograms, allowing one to reliably measure magnitudes for moderate-to-large (M >= 3) earthquakes over broad regions. Because smaller (M < 3) earthquakes are only recorded at higher frequencies for which we find larger interstation scatter, amplitude and magnitude estimates for these events are more variable, regional, and path dependent. In this article, we investigate coda amplitude measurements in the Middle East for 2D variations in attenuation structure. One critical aspect of this effort is characterizing the propagation term to include scattering, which allows us to use amplitudes out to longer distances and later in the coda. We perform a tomographic inversion and find that the recovered attenuation structure is both very similar to the attenuation structure derived from direct phases and also reflective of the tectonic structure of the region. We then apply the 2D attenuation corrections to several hundred events in the region and find marked improvements to our magnitude estimates, as measured by interstation scattering, resulting in standard deviations of less than 0.025 magnitude units at all frequencies. The improvements are greatest at high frequencies, which will have the largest effect on smaller magnitude events.
C1 [Pasyanos, Michael E.; Gok, Rengin; Walter, William R.] Lawrence Livermore Natl Lab, 7000 East Ave,POB 808,L-046, Livermore, CA 94551 USA.
RP Pasyanos, ME (reprint author), Lawrence Livermore Natl Lab, 7000 East Ave,POB 808,L-046, Livermore, CA 94551 USA.
EM pasyanos1@llnl.gov
RI Pasyanos, Michael/C-3125-2013; Walter, William/C-2351-2013
OI Walter, William/0000-0002-0331-0616
FU U.S. Department of Energy by Lawrence Livermore National Laboratory
(LLNL) [DE-AC52-07NA27344]
FX We thank reviewers Mark Fisk and Scott Phillips, and Editor-in-Chief
Diane Doser. We thank Eric Matzel for his assistance in making 1D coda
magnitudes in the Middle East. This work was performed under the
auspices of the U.S. Department of Energy by Lawrence Livermore National
Laboratory (LLNL) under Contract Number DE-AC52-07NA27344. This is LLNL
Contribution Number LLNL-JRNL-679156.
NR 17
TC 1
Z9 1
U1 4
U2 4
PU SEISMOLOGICAL SOC AMER
PI ALBANY
PA 400 EVELYN AVE, SUITE 201, ALBANY, CA 94706-1375 USA
SN 0037-1106
EI 1943-3573
J9 B SEISMOL SOC AM
JI Bull. Seismol. Soc. Amer.
PD OCT
PY 2016
VL 106
IS 5
BP 1915
EP 1925
DI 10.1785/0120150336
PG 11
WC Geochemistry & Geophysics
SC Geochemistry & Geophysics
GA EC8BN
UT WOS:000388365100001
ER
PT J
AU Gok, R
Kaviani, A
Matzel, EM
Pasyanos, ME
Mayeda, K
Yetirmishli, G
El-Hussain, I
Al-Amri, A
Al-Jeri, F
Godoladze, T
Kalafat, D
Sandvol, EA
Walter, WR
AF Gok, Rengin
Kaviani, Ayoub
Matzel, Eric M.
Pasyanos, Michael E.
Mayeda, Kevin
Yetirmishli, Gurban
El-Hussain, Issa
Al-Amri, Abdullah
Al-Jeri, Farah
Godoladze, Tea
Kalafat, Dogan
Sandvol, Eric A.
Walter, William R.
TI Moment Magnitudes of Local/Regional Events from 1D Coda Calibrations in
the Broader Middle East Region
SO BULLETIN OF THE SEISMOLOGICAL SOCIETY OF AMERICA
LA English
DT Article
ID UNITED-STATES EARTHQUAKES; SURROUNDING REGIONS; WAVE-PROPAGATION; LG;
ATTENUATION; SN; SPECTRA; ENERGY
AB Reliable moment magnitude estimates for seismic events in the Middle East region can be difficult to obtain due to the uneven distribution of stations, the complex tectonic structure, and regions of high attenuation. In this study, we take advantage of the many new broadband seismic stations that have become available through improved national networks and numerous temporary deployments. We make coda envelope-amplitude measurements for 2247 events recorded by 68 stations over 13 narrow frequency bands ranging between 0.03 and 8 Hz. The absolute scaling of these spectra was calculated based on independent waveform modeling solutions of the moment magnitudes for a subset of these events to avoid circularity. Using our 1D path calibrations, we determined coda-based magnitudes for a majority of the events. We obtain fairly good agreement with waveform-modeled seismic moments for the larger events (M-w > 4.5) at low frequencies (< 0.7 Hz). As expected, the coda-derived source spectra become increasingly scattered at higher frequencies (> 0.7 Hz) because of unaccounted 2D path effects, as well as mixing of both Sn coda and Lg coda, which have different attenuation behavior. This scatter leads to increased variance in the magnitudes estimated for smaller events in which low-frequency amplitudes are below the noise levels and the higher frequencies are the only signals available. We quantify the expected variance in coda envelope amplitudes as a function of frequency using interstation scatter as our metric. The net results of this study provide thousands of new 1D coda magnitude estimates for events in the broad region, as well as the necessary initial starting model for use in a new related 2D coda study (Pasyanos et al., 2016).
C1 [Gok, Rengin; Matzel, Eric M.; Pasyanos, Michael E.; Walter, William R.] Lawrence Livermore Natl Lab, 7000 East Ave L-049, Livermore, CA 94550 USA.
[Kaviani, Ayoub] Goethe Univ Frankfurt, Inst Geosci, Altenhoeferallee 1, D-60438 Frankfurt, Germany.
[Mayeda, Kevin] Univ Calif Berkeley, EECS, 253 Cory Hall, Berkeley, CA 94720 USA.
[Yetirmishli, Gurban] Natl Acad Sci, Azerbaijan Natl Acad Sci, Republ Seism Survey Ctr Azerbaijan, 25 Nigar Rafibeyli St, AZ-1001 Baku, Azerbaijan.
[El-Hussain, Issa] Sultan Qaboos Univ, Earthquake Monitoring Ctr, POB 50,PC 123, Al Khoud, Oman.
[Al-Amri, Abdullah] King Saud Univ, Riyadh 11451, Saudi Arabia.
[Al-Jeri, Farah] Kuwait Inst Sci Res, POB 24885, Kuwait 13109, Kuwait.
[Godoladze, Tea] Ilia State Univ, Shalva Nutsubidze St, Tbilisi, Rep of Georgia.
[Kalafat, Dogan] Kandilli Observ & Earthquake Res Inst, TR-34684 Istanbul, Turkey.
[Sandvol, Eric A.] Univ Missouri, Dept Geol Sci, 101 Geol Bldg, Columbia, MO 65211 USA.
RP Gok, R (reprint author), Lawrence Livermore Natl Lab, 7000 East Ave L-049, Livermore, CA 94550 USA.
EM gok1@llnl.gov
RI Pasyanos, Michael/C-3125-2013; Yetirmishli, Gurban/C-4257-2017; Walter,
William/C-2351-2013
OI Yetirmishli, Gurban/0000-0002-0542-2443; Walter,
William/0000-0002-0331-0616
FU U.S. Department of Energy by Lawrence Livermore National Laboratory
[DE-AC52-07NA27344]; Air Force Research Laboratory (AFRL)
[FA9453-11-C-0235, DE-AC52-07NA27344/LL11-BAA11-13-NDD03]
FX The majority of the openly available data are obtained from Incorporated
Research Institutions in Seismology (IRIS). Plotting is done using
Generic Mapping Tool (GMT) macros. This work was performed under the
auspices of the U.S. Department of Energy by Lawrence Livermore National
Laboratory under Contract Number DE-AC52-07NA27344. This study is
partially supported by Air Force Research Laboratory (AFRL)
FA9453-11-C-0235 and DE-AC52-07NA27344/LL11-BAA11-13-NDD03. This is
Lawrence Livermore National Laboratory (LLNL) Contribution Number
LLNL-JRNL-679299.
NR 32
TC 1
Z9 1
U1 6
U2 6
PU SEISMOLOGICAL SOC AMER
PI ALBANY
PA 400 EVELYN AVE, SUITE 201, ALBANY, CA 94706-1375 USA
SN 0037-1106
EI 1943-3573
J9 B SEISMOL SOC AM
JI Bull. Seismol. Soc. Amer.
PD OCT
PY 2016
VL 106
IS 5
BP 1926
EP 1938
DI 10.1785/0120160045
PG 13
WC Geochemistry & Geophysics
SC Geochemistry & Geophysics
GA EC8BN
UT WOS:000388365100002
ER
PT J
AU Carmichael, JD
AF Carmichael, Joshua D.
TI A Waveform Detector That Targets Template-Decorrelated Signals and
Achieves Its Predicted Performance, Part I: Demonstration with IMS Data
SO BULLETIN OF THE SEISMOLOGICAL SOCIETY OF AMERICA
LA English
DT Article
ID INTERNATIONAL MONITORING-SYSTEM; CROSS-CORRELATION; NUCLEAR-TEST;
DETECTION CAPABILITY; EVENTS; SEISMICITY; SEQUENCE
AB Waveform correlation detectors used in seismic monitoring scan multi-channel data to test two competing hypotheses: that the data contain (1) a noisy, amplitude-scaled version of a template waveform or (2) only noise. In reality, seismic wavefields include signals triggered by nontarget sources (background seismicity) and target signals that are only partially correlated with the waveform template. We reform the waveform correlation detector hypothesis test to accommodate deterministic uncertainty in template-to-target waveform similarity and thereby derive a new detector from convex set projections (the cone detector) for use in explosion monitoring. Our analyses give probability density functions that quantify the detectors' degraded performance with decreasing waveform similarity. We then apply our results to three announced North Korean nuclear tests and use International Monitoring System (IMS) arrays to determine the probability that low magnitude, off-site explosions can be reliably detected with a given waveform template. We demonstrate that cone detectors provide (1) an improved predictive capability over correlation detectors to identify such spatially separated explosive sources, (2) competitive detection rates, and (3) reduced false alarms on background seismicity.
C1 [Carmichael, Joshua D.] Los Alamos Natl Lab, Bikini Atoll Rd,SM 30, Los Alamos, NM 87544 USA.
RP Carmichael, JD (reprint author), Los Alamos Natl Lab, Bikini Atoll Rd,SM 30, Los Alamos, NM 87544 USA.
FU National Science Foundation (NSF) [1023382]; Department of Energy by Los
Alamos National Security, LLC [DE-AC52-06NA25396]; Office of Nuclear
Detonation Detection [NA-222]
FX I thank two anonymous reviewers who greatly improved the technical
emphasis. Mike Cleveland, Hans Hartse, and Char Rowe improved writing
clarity. Development of initial detection theory work for icequake
analyses was supported by National Science Foundation (NSF) Award
1023382 and Ian Joughin at the University of Washington. The bulk of the
seismic work and application was supported by the Office of Nuclear
Detonation Detection, NA-222. Los Alamos National Laboratory is operated
for the Department of Energy by Los Alamos National Security, LLC, under
Contract DE-AC52-06NA25396.
NR 22
TC 0
Z9 0
U1 3
U2 3
PU SEISMOLOGICAL SOC AMER
PI ALBANY
PA 400 EVELYN AVE, SUITE 201, ALBANY, CA 94706-1375 USA
SN 0037-1106
EI 1943-3573
J9 B SEISMOL SOC AM
JI Bull. Seismol. Soc. Amer.
PD OCT
PY 2016
VL 106
IS 5
BP 1998
EP 2012
DI 10.1785/0120160047
PG 15
WC Geochemistry & Geophysics
SC Geochemistry & Geophysics
GA EC8BN
UT WOS:000388365100008
ER
PT J
AU Arrowsmith, S
Young, C
Ballard, S
Slinkard, M
Pankow, K
AF Arrowsmith, Stephen
Young, Christopher
Ballard, Sanford
Slinkard, Megan
Pankow, Kristine
TI Pickless Event Detection and Location: The Waveform Correlation
Event-Detection System (WCEDS) Revisited
SO BULLETIN OF THE SEISMOLOGICAL SOCIETY OF AMERICA
LA English
DT Article
ID TIME
AB The standard seismic explosion-monitoring paradigm is based on a sparse, spatially aliased network of stations to monitor either the whole Earth or a region of interest. Under this paradigm, state-of-the-art event-detection methods are based on seismic phase picks, which are associated at multiple stations and located using 3D Earth models. Here, we revisit a concept for event-detection that does not require phase picks or 3D models and fuses detection and association into a single algorithm. Our pickless event detector exploits existing catalog and waveform data to build an empirical stack of the full regional seismic wavefield, which is subsequently used to detect and locate events at a network level using correlation techniques. We apply our detector to seismic data from Utah and evaluate our results by comparing them with the earthquake catalog published by the University of Utah Seismograph Stations. The results demonstrate that our pickless detector is a viable alternative technique for detecting events that likely requires less analyst overhead than do the existing methods.
C1 [Arrowsmith, Stephen; Young, Christopher; Ballard, Sanford; Slinkard, Megan] Sandia Natl Labs, POB 5800, Albuquerque, NM 87185 USA.
[Pankow, Kristine] Univ Utah, 115 South 1460 East, Salt Lake City, UT 84112 USA.
RP Arrowsmith, S (reprint author), Sandia Natl Labs, POB 5800, Albuquerque, NM 87185 USA.
EM sjarrow@sandia.gov
FU U.S. Department of Energy; U.S. Department of Energy's National Nuclear
Security Administration [DE-AC04-94AL85000]
FX This research was funded by the U.S. Department of Energy. Sandia
National Laboratories is a multiprogram laboratory managed and operated
by Sandia Corporation, a wholly owned subsidiary of Lockheed Martin
Corporation, for the U.S. Department of Energy's National Nuclear
Security Administration under Contract Number DE-AC04-94AL85000. We are
very grateful to Jim Pechmann and Mark Hale at the University of Utah
Seismograph Stations (UUSS) for answering questions on UUSS algorithms
and catalog results. We thank Rigobert Tibi and Amy Sundermier for their
comments and input. Finally, we thank Associate Editor Ivan Wong and
anonymous reviewers of this article for their valuable feedback.
NR 13
TC 0
Z9 0
U1 0
U2 0
PU SEISMOLOGICAL SOC AMER
PI ALBANY
PA 400 EVELYN AVE, SUITE 201, ALBANY, CA 94706-1375 USA
SN 0037-1106
EI 1943-3573
J9 B SEISMOL SOC AM
JI Bull. Seismol. Soc. Amer.
PD OCT
PY 2016
VL 106
IS 5
BP 2037
EP 2044
DI 10.1785/0120160018
PG 8
WC Geochemistry & Geophysics
SC Geochemistry & Geophysics
GA EC8BN
UT WOS:000388365100011
ER
PT J
AU Graves, R
Pitarka, A
AF Graves, Robert
Pitarka, Arben
TI Kinematic Ground-Motion Simulations on Rough Faults Including Effects of
3D Stochastic Velocity Perturbations
SO BULLETIN OF THE SEISMOLOGICAL SOCIETY OF AMERICA
LA English
DT Article
ID 1979 IMPERIAL-VALLEY; DYNAMIC-RUPTURE MODELS; LOS-ANGELES BASIN;
SAN-ANDREAS FAULT; CRUSTAL HETEROGENEITY; HORIZONTAL COMPONENTS; SOURCE
PARAMETERS; RESPONSE SPECTRA; WAVE-PROPAGATION; SEISMIC-WAVES
AB We describe a methodology for generating kinematic earthquake ruptures for use in 3D ground-motion simulations over the 0-5 Hz frequency band. Our approach begins by specifying a spatially random slip distribution that has a roughly wavenumber-squared fall-off. Given a hypocenter, the rupture speed is specified to average about 75%-80% of the local shear wavespeed and the prescribed slip-rate function has a Kostrov-like shape with a fault-averaged rise time that scales self-similarly with the seismic moment. Both the rupture time and rise time include significant local perturbations across the fault surface specified by spatially random fields that are partially correlated with the underlying slip distribution. We represent velocity-strengthening fault zones in the shallow (< 5 km) and deep (> 15 km) crust by decreasing rupture speed and increasing rise time in these regions. Additional refinements to this approach include the incorporation of geometric perturbations to the fault surface, 3D stochastic correlated perturbations to the P- and S-wave velocity structure, and a damage zone surrounding the shallow fault surface characterized by a 30% reduction in seismic velocity. We demonstrate the approach using a suite of simulations for a hypothetical M-w 6.45 strike-slip earthquake embedded in a generalized hard-rock velocity structure. The simulation results are compared with the median predictions from the 2014 Next Generation Attenuation-West2 Project ground-motion prediction equations and show very good agreement over the frequency band 0.1-5 Hz for distances out to 25 km from the fault. Additionally, the newly added features act to reduce the coherency of the radiated higher frequency (f > 1 Hz) ground motions, and homogenize radiation-pattern effects in this same bandwidth, which move the simulations closer to the statistical characteristics of observed motions as illustrated by comparison with recordings from the 1979 Imperial Valley earthquake.
C1 [Graves, Robert] US Geol Survey, 525 S Wilson Ave, Pasadena, CA 91106 USA.
[Pitarka, Arben] Lawrence Livermore Natl Lab, 7000 East Ave, Livermore, CA 94551 USA.
RP Graves, R (reprint author), US Geol Survey, 525 S Wilson Ave, Pasadena, CA 91106 USA.
EM rwgraves@usgs.gov; pitarka1@llnl.gov
FU National Science Foundation [OCI-0725070, ACI-1238993, OCI-1440085];
state of Illinois; U.S. Department of Energy by Lawrence Livermore
National Laboratory [DE-AC52-07NA27344]
FX Constructive reviews provided by Art Frankel, Elizabeth Cochran, Steve
Day, Steve Hickman, and an anonymous reviewer were very helpful in
revising the article and making it acceptable for publication. Some of
the large-scale computations were performed using the resources of the
Blue Waters sustained-petascale computing project, which is supported by
the National Science Foundation (Awards OCI-0725070 and ACI-1238993) and
the state of Illinois. Blue Waters is a joint effort of the University
of Illinois at Urbana-Champaign and its National Center for
Supercomputing Applications. Access to these resources is also part of
the "Extending the Spatiotemporal Scales of Physics-based Seismic Hazard
Analysis" allocation made to the Southern California Earthquake Center
(SCEC) by the National Science Foundation (Award OCI-1440085). Part of
this work was performed under the auspices of the U.S. Department of
Energy by Lawrence Livermore National Laboratory under Contract Number
DE-AC52-07NA27344. This is SCEC Contribution 6226.
NR 59
TC 0
Z9 0
U1 1
U2 1
PU SEISMOLOGICAL SOC AMER
PI ALBANY
PA 400 EVELYN AVE, SUITE 201, ALBANY, CA 94706-1375 USA
SN 0037-1106
EI 1943-3573
J9 B SEISMOL SOC AM
JI Bull. Seismol. Soc. Amer.
PD OCT
PY 2016
VL 106
IS 5
BP 2136
EP 2153
DI 10.1785/0120160088
PG 18
WC Geochemistry & Geophysics
SC Geochemistry & Geophysics
GA EC8BN
UT WOS:000388365100018
ER
PT J
AU Hirakawa, E
Pitarka, A
Mellors, R
AF Hirakawa, Evan
Pitarka, Arben
Mellors, Robert
TI Generation of Shear Motion from an Isotropic Explosion Source by
Scattering in Heterogeneous Media
SO BULLETIN OF THE SEISMOLOGICAL SOCIETY OF AMERICA
LA English
DT Article
ID FINITE-DIFFERENCE SIMULATIONS; 1997 KAZAKSTAN DEPTH; GROUND-MOTION;
UNDERGROUND EXPLOSIONS; SEISMIC-WAVES; VELOCITY PERTURBATIONS; BURIAL
EXPERIMENT; TECTONIC RELEASE; CODA WAVES; S-WAVES
AB One challenging task in explosion seismology is the development of physical models for explaining the generation of S waves during underground explosions. Recent analysis of ground motion from chemical explosions during the Source Physics Experiment (Pitarka et al., 2015) suggests that, although a large component of shear motion was generated directly at the source, additional scattering from heterogeneous velocity structure and topography is necessary to better match the recorded data. In our study, we used a stochastic representation of small-scale velocity variability to produce high-frequency scattering and to analyze its implication on shear-motion generation during underground explosions. In our stochastic velocity model, the key parameters that affect scattering are the correlation length and the relative amplitude of velocity perturbations. Based on finite-difference simulations of elastic wave propagation from an isotropic explosion source, we find that higher velocity perturbations result in larger shear motion, whereas the correlation length, which controls the scatterers size, affects the frequency range at which relative transverse motion is larger.
C1 [Hirakawa, Evan; Pitarka, Arben; Mellors, Robert] Lawrence Livermore Natl Lab, Atmospher Earth & Energy Div, 7000 East Ave,POB 808 L-046, Livermore, CA 95551 USA.
RP Pitarka, A (reprint author), Lawrence Livermore Natl Lab, Atmospher Earth & Energy Div, 7000 East Ave,POB 808 L-046, Livermore, CA 95551 USA.
EM pitarkaarben@yahoo.com
RI Mellors, Robert/K-7479-2014
OI Mellors, Robert/0000-0002-2723-5163
FU U.S. Department of Energy by Lawrence Livermore National Laboratory
(LLNL) [DE-AC52-07NA27344]
FX We thank Walter Imperatori and the Associate Editor Michel Bouchon for
their careful review and helpful suggestions. We thank Peter Moczo for
insightful discussions about finite-difference methods, and David
Aldridge for sharing with us his findings on wave scattering
simulations. The simulations were performed on the CAB Linux cluster
computer operated by the Livermore Computing center. This work was
performed under the auspices of the U.S. Department of Energy by
Lawrence Livermore National Laboratory (LLNL) under Contract Number
DE-AC52-07NA27344. This is LLNL Contribution Number LLNL-JRNL-676939.
NR 35
TC 0
Z9 0
U1 1
U2 1
PU SEISMOLOGICAL SOC AMER
PI ALBANY
PA 400 EVELYN AVE, SUITE 201, ALBANY, CA 94706-1375 USA
SN 0037-1106
EI 1943-3573
J9 B SEISMOL SOC AM
JI Bull. Seismol. Soc. Amer.
PD OCT
PY 2016
VL 106
IS 5
BP 2313
EP 2319
DI 10.1785/0120150243
PG 7
WC Geochemistry & Geophysics
SC Geochemistry & Geophysics
GA EC8BN
UT WOS:000388365100032
ER
PT J
AU Clark, IC
Youngblut, M
Jacobsen, G
Wetmore, KM
Deutschbauer, A
Lucas, L
Coates, JD
AF Clark, Iain C.
Youngblut, Matt
Jacobsen, Gillian
Wetmore, Kelly M.
Deutschbauer, Adam
Lucas, Lauren
Coates, John D.
TI Genetic dissection of chlorate respiration in Pseudomonas stutzeri PDA
reveals syntrophic (per)chlorate reduction
SO ENVIRONMENTAL MICROBIOLOGY
LA English
DT Article
ID ENTERICA SEROVAR TYPHIMURIUM; DIMETHYL SULFIDE DEHYDROGENASE; NITRATE
REDUCTASE; FLUORESCENT PROTEIN; ELECTRON-TRANSFER; HIGH-THROUGHPUT;
BACTERIAL APBC; SP-NOV; PERCHLORATE; CLUSTER
AB Genes important for growth of Pseudomonas stutzeri PDA on chlorate were identified using a randomly DNA bar-coded transposon mutant library. During chlorate reduction, mutations in genes encoding the chlorate reductase clrABC, predicted molybdopterin cofactor chaperon clrD, molybdopterin biosynthesis and two genes of unknown function (clrE, clrF) had fitness defects in pooled mutant assays (Bar-seq). Markerless in-frame deletions confirmed that clrA, clrB and clrC were essential for chlorate reduction, while clrD, clrE and clrF had less severe growth defects. Interestingly, the key detoxification gene cld was essential for chlorate reduction in isogenic pure culture experiments, but showed only minor fitness defects in Bar-seq experiments. We hypothesized this was enabled through chlorite dismutation by the community, as most strains in the Bar-seq library contained an intact cld. In support of this, Delta cld grew with wild-type PDA or Delta clrA, and purified Cld also restored growth to the Delta cld mutant. Expanding on this, wildtype PDA and a Delta cld mutant of the perchlorate reducer Azospira suillum PS grew on perchlorate in co-culture, but not individually. These results demonstrate that co-occurrence of cld and a chloroxyanion reductase within a single organism is not necessary and raises the possibility of syntrophic (per) chlorate respiration in the environment.
C1 [Clark, Iain C.] Univ Calif Berkeley, Dept Civil & Environm Engn, Berkeley, CA 94720 USA.
[Youngblut, Matt; Jacobsen, Gillian; Lucas, Lauren; Coates, John D.] Univ Calif Berkeley, Plant & Microbial Biol, Berkeley, CA 94720 USA.
[Wetmore, Kelly M.; Deutschbauer, Adam] Lawrence Berkeley Natl Lab, Phys Biosci Div, Berkeley, CA USA.
RP Coates, JD (reprint author), Univ Calif Berkeley, Plant & Microbial Biol, Berkeley, CA 94720 USA.
EM jdcoates@berkeley.edu
FU Energy Biosciences Institute, University of California, Berkeley; NIH
[S10RR029668, S10RR027303]
FX Thanks to Morgan Price for insight into pooled mutant fitness assays and
for sharing the computational framework used to analyse Bar-seq
experiments. Funding for research on perchlorate and chlorate reduction
in the laboratory of J.D.C. has been provided through the Energy
Biosciences Institute, University of California, Berkeley. The funders
had no role in study design, data collection and analysis, decision to
publish or preparation of the manuscript. This work used the Vincent J.
Coates Genomics Sequencing Laboratory at UC Berkeley, supported by NIH
S10 Instrumentation Grants S10RR029668 and S10RR027303. The
Computational Genomics Resource Laboratory, which is part of the
California Institute for Quantitative Biosciences, was for used for
computational analysis. The authors declare no conflict of interest.
NR 57
TC 3
Z9 3
U1 0
U2 0
PU WILEY-BLACKWELL
PI HOBOKEN
PA 111 RIVER ST, HOBOKEN 07030-5774, NJ USA
SN 1462-2912
EI 1462-2920
J9 ENVIRON MICROBIOL
JI Environ. Microbiol.
PD OCT
PY 2016
VL 18
IS 10
SI SI
BP 3342
EP 3354
DI 10.1111/1462-2920.13068
PG 13
WC Microbiology
SC Microbiology
GA ED1NW
UT WOS:000388613200012
PM 26411776
ER
PT J
AU Summerscales, OT
Batista, ER
Scott, BL
Wilkerson, MP
Sutton, AD
AF Summerscales, Owen T.
Batista, Enrique R.
Scott, Brian L.
Wilkerson, Marianne P.
Sutton, Andrew D.
TI Reversible Formation of a Cerium-Bound Terminal Hydride:
Ce(C5Me4SiMe3)(2)(H)(thf)
SO EUROPEAN JOURNAL OF INORGANIC CHEMISTRY
LA English
DT Article
DE Hydrides; C-H activation; Lanthanides; Cerium
ID C-H ACTIVATION; FLUORINE EXCHANGE; CRYSTAL-STRUCTURE; BOND METATHESIS;
COMPLEXES; HYDROGEN; DERIVATIVES; LANTHANIDE; CHEMISTRY; ELEMENTS
AB The use of the bulky cyclopentadienyl ligand Cp' (Cp' = C5Me4SiMe3) to stabilize cerium hydrides has resulted in the preparation of two novel tuck-in complexes with C-H activated SiMe3 groups. Subsequent reaction of these with H-2 in thf gives a lanthanide terminal hydride species Ce(Cp')(2)(H)(thf) which reversibly regenerates the tuck-in complex under sustained vacuum. This compound is only the second structurally characterized terminal cerium hydride. This new hydride is a catalyst in H/D exchange reactions between with both sp(3)-CH and sp(2)-CH bonds, and for the hydrogenation of unsaturated alkene bonds.
C1 [Summerscales, Owen T.; Wilkerson, Marianne P.; Sutton, Andrew D.] Los Alamos Natl Lab, Div Chem, Los Alamos, NM 87545 USA.
[Batista, Enrique R.] Los Alamos Natl Lab, Div Theoret, Los Alamos, NM 87545 USA.
[Scott, Brian L.] Los Alamos Natl Lab, Mat & Phys Applicat Div, Los Alamos, NM 87545 USA.
RP Sutton, AD (reprint author), Los Alamos Natl Lab, Div Chem, Los Alamos, NM 87545 USA.
EM adsutton@lanl.gov
RI Sutton, Andrew/D-1047-2015; Scott, Brian/D-8995-2017
OI Sutton, Andrew/0000-0001-7984-1715; Scott, Brian/0000-0003-0468-5396
FU Los Alamos National Laboratory LDRD-DR (Laboratory Directed Research and
Development - Directed Research); U.S. Department of Energy
[DE-AC5206NA25396]
FX This work was funded by Los Alamos National Laboratory LDRD-DR
(Laboratory Directed Research and Development - Directed Research). Los
Alamos National Laboratory is operated by Los Alamos National Security,
LLC, for the National Nuclear Security Administration of the U.S.
Department of Energy under contract DE-AC5206NA25396.
NR 25
TC 2
Z9 2
U1 2
U2 2
PU WILEY-V C H VERLAG GMBH
PI WEINHEIM
PA POSTFACH 101161, 69451 WEINHEIM, GERMANY
SN 1434-1948
EI 1099-0682
J9 EUR J INORG CHEM
JI Eur. J. Inorg. Chem.
PD OCT
PY 2016
IS 28
BP 4551
EP 4556
DI 10.1002/ejic.201600737
PG 6
WC Chemistry, Inorganic & Nuclear
SC Chemistry
GA DZ9CA
UT WOS:000386169600004
ER
PT J
AU Oswald, BP
Dugan, SC
Balice, RG
Unger, DR
AF Oswald, Brian P.
Dugan, Sean C.
Balice, Randy G.
Unger, Daniel R.
TI Overstory Tree Mortality in Ponderosa Pine and Spruce-Fir Ecosystems
Following a Drought in Northern New Mexico
SO FORESTS
LA English
DT Article
DE aspen; white fir; Douglas-fir; succession; Jemez Mountains
ID FORESTS; DEATH
AB Drought-caused tree dieback is an issue around the world as climates change and many areas become dryer and hotter. A drought from 1998-2004 resulted in a significant tree dieback event in many of the wooded areas in portions of the Jemez Mountains and the adjacent Pajarito Plateau in northern New Mexico. The objectives of this study were to evaluate and quantify the differences in tree mortality before and after a recent drought in ponderosa pine and spruce-fir ecosystems, and to assess the effect of mechanical thinning on ponderosa pine mortality. Significant increases in mortality were observed in the unthinned ponderosa pine ecosystem. Mortality varied significantly between species and within size classes. Mechanical thinning of ponderosa pines reduced overstory mortality to non-significant levels. A lack of rainfall, snowfall, and increases in daily minimum temperature contributed most to the mortality. Adaptive management, including the use of thinning activities, appear to moderate the impact of climate change on ponderosa pine forests in this region, increasing the long-term health of the ecosystem. The impact of climate change on the spruce-fir ecosystems may accelerate successional changes.
C1 [Oswald, Brian P.; Unger, Daniel R.] Stephen F Austin State Univ, Arthur Temple Coll Forestry & Agr, POB 6109 SFA Stn, Nacogdoches, TX 75962 USA.
[Dugan, Sean C.] Big Bend Ranch State Pk Texas Pk & Wildlife, 1900 Sauceda Ranch Rd, Presidio, TX 79845 USA.
[Balice, Randy G.] Los Alamos Natl Lab, Los Alamos, NM 87545 USA.
RP Oswald, BP (reprint author), Stephen F Austin State Univ, Arthur Temple Coll Forestry & Agr, POB 6109 SFA Stn, Nacogdoches, TX 75962 USA.
EM boswald@sfasu.du; Scdugan53@gmail.com; balice@lanl.gov; unger@sfasu.edu
FU Division of Environmental Science in the Arthur Temple College of
Forestry and Agriculture at Stephen F. Austin State University
FX We thank Scot Johnson, the Environmental Data and Analysis Group Leader,
at Los Alamos National Laboratory for the meteorological data and the
Division of Environmental Science in the Arthur Temple College of
Forestry and Agriculture at Stephen F. Austin State University for
financial support. We also thank anonymous reviewers for their
recommendations to improve this manuscript.
NR 22
TC 0
Z9 0
U1 4
U2 4
PU MDPI AG
PI BASEL
PA ST ALBAN-ANLAGE 66, CH-4052 BASEL, SWITZERLAND
SN 1999-4907
J9 FORESTS
JI Forests
PD OCT
PY 2016
VL 7
IS 10
AR 225
DI 10.3390/f7100225
PG 16
WC Forestry
SC Forestry
GA ED2JQ
UT WOS:000388670800016
ER
EF