Author: "Department of Physics [Gainesville] (UF|Physics)" - Searchworks@Jio Institute Digital Library Search Results

19 results on '"Department of Physics [Gainesville] (UF|Physics)"'

1. Prompt gravity signal induced by the 2011 Tohoku-Oki earthquake

Author: Jan Harms, Bernard F. Whiting, M. Barsuglia, E. Chassande-Mottin, Kévin Juhel, Pascal Bernard, Philippe Lognonné, Jean-Paul Montagner, Eric Clévédé, Jean-Paul Ampuero, Institut de Physique du Globe de Paris (IPGP), Institut national des sciences de l'Univers (INSU - CNRS)-IPG PARIS-Université Paris Diderot - Paris 7 (UPD7)-Université de La Réunion (UR)-Centre National de la Recherche Scientifique (CNRS), AstroParticule et Cosmologie (APC (UMR_7164)), Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Seismological Laboratory, California Institute of Technology, 1200 E. California Blvd., Pasadena, California 91125, USA., National Institute for Nuclear Physics, Sezione Firenze, Via G Sansone 1, Sesto Fiorentino, 50019 and Universita` degli Studi di Urbino ‘‘Carlo Bo‘‘, I-61029 Urbino, Italy, Department of Physics [Gainesville] (UF|Physics), University of Florida [Gainesville] (UF), Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-IPG PARIS-Université Paris Diderot - Paris 7 (UPD7)-Université de La Réunion (UR)-Centre National de la Recherche Scientifique (CNRS), Centre National de la Recherche Scientifique (CNRS)-Université de La Réunion (UR)-Université Paris Diderot - Paris 7 (UPD7)-IPG PARIS-Institut national des sciences de l'Univers (INSU - CNRS), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7), Department of Physics, 2001 Museum Road, University of Florida, Gainesville, Florida 32611-8440, USA, Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris Diderot - Paris 7 (UPD7)-Université de La Réunion (UR)-Institut de Physique du Globe de Paris (IPG Paris)-Centre National de la Recherche Scientifique (CNRS), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), and Università degli Studi di Urbino 'Carlo Bo'
Subjects: Seismometer, Peak ground acceleration, Multidisciplinary, 010504 meteorology & atmospheric sciences, Gravimeter, Science, [SDU.STU]Sciences of the Universe [physics]/Earth Sciences, General Physics and Astronomy, Supershear earthquake, General Chemistry, Seismic noise, 010502 geochemistry & geophysics, 01 natural sciences, General Biochemistry, Genetics and Molecular Biology, Seismic wave, Article, Physics::Geophysics, Earthquake simulation, [SDU]Sciences of the Universe [physics], Earthquake rupture, Seismology, Geology, 0105 earth and related environmental sciences
Abstract: Transient gravity changes are expected to occur at all distances during an earthquake rupture, even before the arrival of seismic waves. Here we report on the search of such a prompt gravity signal in data recorded by a superconducting gravimeter and broadband seismometers during the 2011 Mw 9.0 Tohoku-Oki earthquake. During the earthquake rupture, a signal exceeding the background noise is observed with a statistical significance higher than 99% and an amplitude of a fraction of μGal, consistent in sign and order of magnitude with theoretical predictions from a first-order model. While prompt gravity signal detection with state-of-the-art gravimeters and seismometers is challenged by background seismic noise, its robust detection with gravity gradiometers under development could open new directions in earthquake seismology, and overcome fundamental limitations of current earthquake early-warning systems imposed by the propagation speed of seismic waves., Earthquakes have been theorised to produce gravity signals that may arrive before seismic waves, but until now they had not been detected. Montagner et al. have detected prompt gravity signals from the 2011 Tohoku-Oki earthquake thus allowing an early warning of earthquakes before seismic wave arrival.
Published: 2016

2. Earthquake early warning using future generation gravity strainmeters

Author: Jan Harms, J. P. Montagner, Martin Vallée, Pascal Bernard, M. Barsuglia, E. Chassande-Mottin, Kévin Juhel, B. F. Whiting, D. Fiorucci, Jean-Paul Ampuero, AstroParticule et Cosmologie (APC (UMR_7164)), Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Institut de Physique du Globe de Paris (IPGP), Centre National de la Recherche Scientifique (CNRS)-Université de La Réunion (UR)-Université Paris Diderot - Paris 7 (UPD7)-IPG PARIS-Institut national des sciences de l'Univers (INSU - CNRS), Géoazur (GEOAZUR 7329), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de la Côte d'Azur, COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD [France-Sud]), Institut de Recherche pour le Développement (IRD), Istituto Nazionale di Fisica Nucleare, Sezione di Firenze (INFN, Sezione di Firenze), Istituto Nazionale di Fisica Nucleare (INFN), Department of Physics [Gainesville] (UF|Physics), University of Florida [Gainesville] (UF), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris Diderot - Paris 7 (UPD7)-Université de La Réunion (UR)-Institut de Physique du Globe de Paris (IPG Paris)-Centre National de la Recherche Scientifique (CNRS), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7), Institut national des sciences de l'Univers (INSU - CNRS)-Institut de Recherche pour le Développement (IRD [France-Sud])-Centre National de la Recherche Scientifique (CNRS)-Observatoire de la Côte d'Azur, Université Côte d'Azur (UCA)-Université Côte d'Azur (UCA), National Institute for Nuclear Physics (INFN), Department of Physics [Gainesville], and University of Florida [Gainesville]
Subjects: Seismometer, [PHYS]Physics [physics], 010504 meteorology & atmospheric sciences, Warning system, Subduction, Gravimeter, [SDU.STU]Sciences of the Universe [physics]/Earth Sciences, 010502 geochemistry & geophysics, Gravitational acceleration, Geodesy, 01 natural sciences, Seismic wave, Geophysics, 13. Climate action, Space and Planetary Science, Geochemistry and Petrology, Homogeneous, Earth and Planetary Sciences (miscellaneous), Astronomical interferometer, Geology, 0105 earth and related environmental sciences
Abstract: Recent studies reported the observation of prompt elastogravity signals during the 2011 M9.1 Tohoku earthquake, recorded with broadband seismometers and gravimeter between the rupture onset and the arrival of the seismic waves. Here we show that to extend the range of magnitudes over which the gravity perturbations can be observed and reduce the time needed for their detection, high-precision gravity strainmeters under development could be used, such as torsion bars, superconducting gradiometers or strainmeters based on atom interferometers. These instruments measure the differential gravitational acceleration between two seismically isolated test masses, and are designed to observe signals around 0.1 Hz. We show that these instruments should be able to detect prompt gravity perturbations induced by earthquakes larger than M7, up to 1000 km from the earthquake centroid within P-waves travel time and up to 120 km within the first 10 seconds of rupture onset, provided a sensitivity in gravity strain of 10^{-15} Hz^{-1/2} at 0.1 Hz can be achieved. The analysis involves simulations of the expected gravity strain signals based on an analytical model of gravity perturbations generated by fault rupture in a homogeneous half-space. As an immediate application, we discuss the possibility to improve current earthquake-early warning systems (EEWS). Our results suggest that, in comparison to conventional P-wave-based EEWS, a gravity-based warning system could perform faster detections of large off-shore subduction earthquakes (at least larger than M7.4). Gravity strainmeters could also perform earlier magnitude estimates, within the duration of the fault rupture, and therefore complement current tsunami warning systems.
Published: 2018

3. Using controlled disorder to probe the interplay between charge order and superconductivity in NbSe$_2$

Author: Makariy A. Tanatar, Robert J. McQueeney, Vivek Mishra, P. B. Gartin, Kyuil Cho, Alan I. Goldman, John Wilde, Serafim Teknowijoyo, J. P. Guss, Peter Hirschfeld, Ruslan Prozorov, Marcin Konczykowski, Andreas Kreyssig, The Ames Laboratory (Ameslab), Iowa State University (ISU)-U.S. Department of Energy, Laboratoire des Solides Irradiés (LSI), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Centre National de la Recherche Scientifique (CNRS)-École polytechnique (X), Department of Microsystems Engineering [Freiburg] (IMTEK), University of Freiburg [Freiburg], Department of Physics and Astronomy [Ames, Iowa], Iowa State University (ISU), Laboratoire de physique des gaz et des plasmas (LPGP), Université Paris-Sud - Paris 11 (UP11)-Centre National de la Recherche Scientifique (CNRS), Computer Science and Mathematics Division [Oak Ridge], Oak Ridge National Laboratory [Oak Ridge] (ORNL), UT-Battelle, LLC-UT-Battelle, LLC, Department of Physics [Gainesville] (UF|Physics), University of Florida [Gainesville] (UF), and Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-École polytechnique (X)-Centre National de la Recherche Scientifique (CNRS)
Subjects: Science, London penetration depth, General Physics and Astronomy, FOS: Physical sciences, 02 engineering and technology, 01 natural sciences, General Biochemistry, Genetics and Molecular Biology, Article, Superconductivity (cond-mat.supr-con), Electrical resistivity and conductivity, Condensed Matter::Superconductivity, 0103 physical sciences, Electron beam processing, Irradiation, 010306 general physics, lcsh:Science, Superconductivity, Physics, [PHYS]Physics [physics], Multidisciplinary, Condensed matter physics, Scattering, Condensed Matter - Superconductivity, Charge (physics), General Chemistry, 021001 nanoscience & nanotechnology, Pairing, Condensed Matter::Strongly Correlated Electrons, lcsh:Q, 0210 nano-technology
Abstract: The interplay between superconductivity and charge-density wave (CDW) in 2H-NbSe2 is not fully understood despite decades of study. Artificially introduced disorder can tip the delicate balance between two competing long-range orders, and reveal the underlying interactions that give rise to them. Here we introduce disorder by electron irradiation and measure in-plane resistivity, Hall resistivity, X-ray scattering, and London penetration depth. With increasing disorder, the superconducting transition temperature, Tc, varies non-monotonically, whereas the CDW transition temperature, TCDW, monotonically decreases and becomes unresolvable above a critical irradiation dose where Tc drops sharply. Our results imply that the CDW order initially competes with superconductivity, but eventually assists it. We argue that at the transition where the long-range CDW order disappears, the cooperation with superconductivity is dramatically suppressed. X-ray scattering and Hall resistivity measurements reveal that the short-range CDW survives above the transition. Superconductivity persists to much higher dose levels, consistent with fully gapped superconductivity and moderate interband pairing., The interplay between superconductivity and charge density wave (CDW) in 2H-NbSe2 is still not fully understood. Here, Cho et al. use controlled disorder to probe the interplay between these two phases in 2H-NbSe2 and find that superconductivity initially competes with CDW but eventually long-range CDW order assists superconductivity.
Published: 2018

4. Differentiation of Surface and Bulk Conductivities in Topological Insulators via Four-Probe Spectroscopy

Author: Yong P. Chen, Saban M. Hus, Chuanxu Ma, Michael A. McGuire, Ireneusz Miotkowski, Helin Cao, An-Ping Li, Corentin Durand, Yang Xu, Xiaoguang Zhang, Center for Nanophase Materials Sciences [Oak Ridge] (CNMS), Oak Ridge National Laboratory [Oak Ridge] (ORNL), UT-Battelle, LLC-UT-Battelle, LLC, Department of Physics [Gainesville] (UF|Physics), and University of Florida [Gainesville] (UF)
Subjects: Materials science, Condensed matter physics, Graphene, Mechanical Engineering, Conductance, Bioengineering, 02 engineering and technology, General Chemistry, 021001 nanoscience & nanotechnology, Condensed Matter Physics, Thermal conduction, 01 natural sciences, law.invention, law, Topological insulator, 0103 physical sciences, [PHYS.COND.CM-MS]Physics [physics]/Condensed Matter [cond-mat]/Materials Science [cond-mat.mtrl-sci], General Materials Science, Scanning tunneling microscope, 010306 general physics, 0210 nano-technology, Spectroscopy, Scaling, Surface states
Abstract: International audience; We show a new method to differentiate conductivities from the surface states and the coexisting bulk states in topological insulators using a four-probe transport spectroscopy in a multiprobe scanning tunneling microscopy system. We derive a scaling relation of measured resistance with respect to varying interprobe spacing for two interconnected conduction channels to allow quantitative determination of conductivities from both channels. Using this method, we demonstrate the separation of 2D and 3D conduction in topological insulators by comparing the conductance scaling of Bi2Se3, Bi2Te2Se, and Sb-doped Bi2Se3 against a pure 2D conductance of graphene on SiC substrate. We also quantitatively show the effect of surface doping carriers on the 2D conductance enhancement in topological insulators. The method offers a means to understanding not just the topological insulators but also the 2D to 3D crossover of conductance in other complex systems.
Published: 2016

5. All-sky search for long-duration gravitational wave transients in the first Advanced LIGO observing run

Author: L. Sammut, S. Appert, G. Pillant, Rakesh Kumar, J. Warner, J. C. Driggers, Gor Oganesyan, P. J. Quinonez, A. Schönbeck, B. Rajbhandari, L. Pinard, A. M. Holgado, Olivier Minazzoli, Sebastiano Bernuzzi, B. Lantz, Daniel Wysocki, Abhirup Ghosh, D. Meacher, M. Razzano, B. Grace, S. M. Aronson, J. L. Willis, M. J. Szczepańczyk, S. J. Kapadia, J. M. Gonzalez Castro, P. J. Easter, L. M. DeMarchi, Chunglee Kim, F. Carbognani, D. Barta, J. S. Kissel, H. Cao, D. J. Vine, M. Favata, Roger Jones, V. J. Roma, A. P. Spencer, D. D. Brown, M. Fyffe, Anthony A. Amato, N. van Bakel, Yichen Huang, K. Lee, A. Masserot, K. Kawabe, S. M. Aston, K. Ueno, Michael W. Coughlin, F. Frasconi, O. Halim, M. Fitz-Axen, J. D. Jones, M. Merzougui, S. J. Jadhav, P. Bacon, Daniel E. Holz, Z. Yang, V. Avendano, A. L. Stuver, H. K. Lee, L. Kleybolte, Torrey Cullen, K. Siellez, J. Oberling, Karan Jani, K. W. Tsang, A. C. Green, G. Vedovato, S. J. Chamberlin, S. Hochheim, A. R. Williamson, F. Muciaccia, Lionel London, P. Oppermann, R. Mittleman, Steven Bloemen, Jonathan R. Gair, H. A. G. Gabbard, A. Dasgupta, Charalampos Markakis, Karl Gill, V. Srivastava, Nelson Christensen, D. Laghi, S. A. Usman, R. Shink, E. Goetz, Huang-Wei Pan, Gijs Nelemans, N. V. Keerthana, Fausto Acernese, H. S. Cho, N. A. Robertson, F. Nocera, E. D. Hall, M. Cieślar, Bernard F. Whiting, M. Kasprzack, M. Fays, B. Idzkowski, V. Loriette, Marco Romanelli, V. Skliris, E. Payne, L. Conti, C. Gray, G. H. Ogin, B. Patricelli, S. S. Eikenberry, Serena Vinciguerra, K. E. Ramirez, R. Pedurand, Benno Willke, M. Rakhmanov, Nicolas Sanchis-Gual, G. Koekoek, Jolien D. E. Creighton, D. Huet, S. H. Huttner, O. J. Piccinni, D. Singh, M. Mantovani, David Jonathan Hofman, Michael E Zucker, A. Sur, Mairi Sakellariadou, M. Nery, Benjamin J. Owen, J. F. J. van den Brand, Archisman Ghosh, D. Moffa, Jocelyn Read, M. P. Ross, K. S. Phukon, Michela Mapelli, J. Li, X. Liu, S. H. R. Yuen, N. Radulesco, J. Eichholz, J. J. McCann, T. J. Slaven-Blair, S. ShyamSundar, C. Stachie, P. Ehrens, S. Sunil, M. Tacca, Martin Hendry, Cecilio García-Quirós, R. Flaminio, S. P. Stevenson, J.-P. Coulon, J. Hennig, Ettore Majorana, A. Di Lieto, D. S. Wu, Margaret Millhouse, S. G. Gaonkar, V. Boschi, R. J. G. Jonker, Jay D. Tasson, O. de Varona, M. Landry, M. Saleem, Marcus E. Lower, R. Prasanna, D. Steinmeyer, A. Tripathee, L. Di Fiore, Jonathan Blackman, Haixing Miao, H. Ohta, Piotr Jaranowski, V. Gayathri, S. Walsh, Miriam Cabero, Alessandra Buonanno, R. Metzdorff, B. D. Lackey, Sebastien Biscans, D. H. Reitze, A. Grimaldi, F. Di Giovanni, B. Mours, S. A. Nichols, F. Meylahn, C. Austin, T. Shaffer, D. Pascucci, C. Bradaschia, Gabriela Gonzalez, K. R. Corley, I. Belahcene, Jonathan Cripe, K. Toland, M. Boer, H. Fong, V. Bossilkov, James G. Bartlett, M. Barsuglia, A. K. Y. Li, David Jones, Paul M. Ricker, F. Cleva, Andrew Melatos, M. Lorenzini, Marco Cavaglia, Tenglin Li, C. Buy, Christopher Wipf, M. C. Díaz, Antonios Kontos, L. Trozzo, H. Yamamoto, Gabrielle Allen, J.-M. Isac, Carlos O. Lousto, C. North, Thomas Dent, P. Corban, Junwei Cao, S. Grunewald, S. Sitmukhambetov, K. L. Dooley, Aaron Zimmerman, Kazuhiro Agatsuma, Y. Boetzel, Odylio D. Aguiar, Maximiliano Isi, M. Croquette, E. M. Gretarsson, Ying Guo, D. Beniwal, Peter Fritschel, Wenxiao Wang, D. Estevez, B. L. Swinkels, A. Cirone, K. Merfeld, J. Jiang, D. H. Shoemaker, J. Junker, A. Kumar, Miguel-Ángel Aloy, José A. Font, N. Singh, James Healy, Kevin M. Ryan, C. Difronzo, F. Vetrano, Shreya Anand, Hyang Woon Lee, Maya Fishbach, Ryan Lynch, Lei Zhang, L. E. H. Datrier, S. Mastrogiovanni, F. Morawski, M. Bejger, R. K. Lanza, Fangchen Feng, James Whelan, P. Ajith, S. D'Antonio, M. Bitossi, J. H. Briggs, J. Calderón Bustillo, A. Sergeev, D. J. McManus, M. Masso-Reid, M. Tonelli, P. Clearwater, E. J. Fauchon-Jones, H. Overmier, M. J. Cowart, D. Stocks, Subroto Mukherjee, Edward K. Porter, Lisa Barsotti, G. Kang, A. Chiummo, J. H. Klika, O. Sauter, V. Hui, J. H. Romie, C. C. Yancey, R. L. McCarthy, Michael Zevin, P. Dupej, F. Marion, P. Grassia, Kipp Cannon, Luca Gammaitoni, Eric B. Flynn, S. Ponrathnam, Chunnong Zhao, S. A. Bilgili, K. Wette, J. Brooks, M. Drago, J. Meidam, M. Steinke, M. Muratore, A. F. Brooks, P. G. Murray, Francesco Pannarale, M. C. Milovich-Goff, Roman Schnabel, A. Lenon, C. Messenger, X. Fan, Bruno Giacomazzo, Soichiro Morisaki, Tanja Hinderer, John J. Oh, J. L. Wright, Timothy Evans, Sascha Husa, M. Vardaro, G. Venugopalan, D.B. DeBra, A. Strunk, B. Gateley, E. Maros, Aaron Buikema, R. Frey, Pablo Cerdá-Durán, Vivien Raymond, K.S.J. Rao, J. Betzwieser, Francesco Chiadini, D. J. Stops, R. L. Savage, J. E. Brau, A. A. van Veggel, Guoying Zhao, Guenakh Mitselmakher, P. Fulda, H. M. Lee, L. Wallace, J. Petermann, Patrick Godwin, P. Brockill, Efim A. Khazanov, G. Ballardin, A. Lazzarini, N. Leroy, A. Rocchi, C. Krämer, B. Bécsy, B. K. Berger, F. Ohme, J. Scott, A. Ain, B. A. Boom, M. G. Benjamin, Des Gibson, B. Goncharov, R. Birney, D. M. Wilken, A. Mullavey, Marie-Anne Bizouard, H. Estelles, L. Cunningham, Sheelu Abraham, V. Kringel, P. T.H. Pang, E. J. Daw, M. Punturo, Mandar Patil, Zhihui Du, G. Ciani, A. Parida, A. Dmitriev, R. Passaquieti, O. Durante, Rory Smith, C. Adams, W. A. Campbell, J. S. H. Lee, D. Sigg, R. Tso, M. Kovalam, Felix Wellmann, S. E. Barclay, M. Eisenmann, Ofek Birnholtz, N. N. Janthalur, P. H. Nguyen, Antonio Marquina, Peter R. Saulson, J. Prasad, Karsten Danzmann, Andrea H. Tapia, Vivishek Sudhir, E. Schreiber, Elton J. G. Santos, W. G. Anderson, G. Mo, G. Cella, T. A. Ferreira, Samaya Nissanke, L. Terkowski, Leo Singer, M. K. M. Bader, R. A. Mercer, K. D. Giardina, A. Brillet, S. Katsanevas, Hua Wang, G. Cho, L. Mereni, Patrick M. Koch, S. Antier, S. W. Ballmer, D. M. Shoemaker, T. Huynh-Dinh, O. Chaibi, J. A. Clark, M. Wade, Srishti Tiwari, C. Lazzaro, T. Z. Summerscales, Patricia Schmidt, A. Avila-Alvarez, A. S. Markosyan, S. Banagiri, S. Frasca, T. L. Lam, S. D. Linker, P. Hopkins, J. K. Wofford, Eric Howell, M. A. Page, F. Magaña-Sandoval, Hartmut Grote, T. P. Downes, Jonathan Richardson, Mark A. Scheel, X. Li, A. K. Zadrożny, R. De Rosa, Podila Satya Venkata Narasimha Sharma, B. P. Abbott, Terry G. McRae, C. Rajan, P. Leaci, V. Sequino, E. K. Gustafson, R. P. Fisher, S. Mitra, M. Standke, Rosa Poggiani, Slawomir Gras, J. Hanson, V. Frey, A. K. Mehta, M. C. Tringali, I. Nardecchia, Monica Colpi, Lloyd Paul Aiello, B. C. Pant, Tomasz Bulik, Ryan Magee, Andrew Lundgren, Alessandro Longo, D. Fiorucci, Richard J. Oram, S. Xiao, W. S. Kim, Nergis Mavalvala, L. E. Sanchez, S. Leavey, Hai-Ping Cheng, A. Iess, S. W. S. Ng, J. S. Lange, G. Losurdo, G. G. Fronzé, S. V. Angelova, Michelle E. Walker, J. George, Kai Staats, C. Nguyen, K. Prasai, Jerome Degallaix, Isabel Cordero-Carrión, S. Meshkov, A. Bozzi, L. G. Prokhorov, Otto A. Hannuksela, Albino Perego, Y. K. Lecoeuche, Samuele Cortese, H. Qi, Charlie Hoy, B. R. Hall, S. Doravari, M. Chaturvedi, C. Casentini, Gregory M. Harry, G. Moreno, H. Inchauspe, Linqing Wen, C. J. Richardson, François Bondu, J. R. Palamos, Sourav Ghosh, Imre Bartos, Enrico Calloni, Nandita Khetan, S. Soni, F. Badaracco, M. Haney, S. Vass, T. Dal Canton, S. Farinon, M. Constancio, E. Mejuto Villa, B. B. Lane, A. Pele, M. Bawaj, A. Mishkin, A. Ramos-Buades, Thomas Corbitt, B. Irwin, J. Liu, L. K. Nuttall, D. Tuyenbayev, Maria Ilaria Del Principe, N. V. Krishnendu, F. Y. Khalili, R. DeSalvo, D. Sellers, F. Lin, R. Coyne, P. Puppo, Fabrice Matichard, R. Cotesta, Yuri Levin, M. Agathos, V. Martinez, P. J. Veitch, Daniele A. Steer, Denis Martynov, P. Booker, Prafulla K. Panda, V. Quetschke, L. Salconi, Antoine Heidmann, S. G. Crowder, Devon S. Johnson, Stephen Fairhurst, Carl Blair, T. Sadecki, R. Macas, F. Travasso, J. Bosveld, G. Billingsley, S. Macfoy, Tania Regimbau, M. Arène, B. U. Gadre, R. M. S. Schofield, Neil J. Cornish, W. Parker, A. Macquet, S. B. Anderson, M. Mondin, Archana Pai, R. Sturani, F. Paoletti, Innocenzo M. Pinto, C. Horst, Alberto Vecchio, D. M. Macleod, Tim Dietrich, Harald P. Pfeiffer, J. Gniesmer, Robert Stone, Marco Bazzan, O. V. Palashov, Sean T. McWilliams, C. Ingram, A. Kutynia, Alessandro Nagar, J. M. Fishner, F. Martelli, B. R. Iyer, D. Töyrä, G. M. Guidi, Martin M. Fejer, J. R. Smith, S. Ghonge, E. A. Huerta, M. C. Heintze, K. li, C. Fee, David Coward, A. Miani, M. Rizzo, I. W. Martin, M. Zanolin, B. Weaver, E. J. Son, C. A. Costa, V. Kondrashov, F. Piergiovanni, Will M. Farr, M. Montani, Chang-Hwan Lee, Rana X. Adhikari, R. Goetz, Nancy Aggarwal, Yang Yang, S. L. Danilishin, Arunava Mukherjee, T. J. N. Nelson, Silvia Corezzi, Om Sharan Salafia, G. Bergmann, V. Tiwari, Wolfango Plastino, K. AultONeal, Carl-Johan Haster, L. Rolland, C. L. Romel, C. S. Unnikrishnan, Richard O'Shaughnessy, B. Barr, Fabrizio Barone, M. T. Hübner, Mark Thomas, N. Man, G. Eddolls, Erik Katsavounidis, D. Sentenac, S. Bae, David B. 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Sciences et Technologies (UMR 6174) (FEMTO-ST), Université de Technologie de Belfort-Montbeliard (UTBM)-Ecole Nationale Supérieure de Mécanique et des Microtechniques (ENSMM)-Université de Franche-Comté (UFC), Université Bourgogne Franche-Comté [COMUE] (UBFC)-Université Bourgogne Franche-Comté [COMUE] (UBFC)-Centre National de la Recherche Scientifique (CNRS), Hulleras del Norte, S.A., European gravitational Observatory (EGO), Istituto Nazionale di Fisica Nucleare (INFN)-Centre National de la Recherche Scientifique (CNRS), School of Electrical and Computer Engineering - Georgia Insitute of Technology (ECE GeorgiaTech), Georgia Institute of Technology [Atlanta], Imagerie Ultrasonore, Centre de Recherche en Acquisition et Traitement de l'Image pour la Santé (CREATIS), Université Jean Monnet [Saint-Étienne] (UJM)-Hospices Civils de Lyon (HCL)-Institut National des Sciences Appliquées de Lyon (INSA Lyon), Université de Lyon-Institut National des Sciences Appliquées (INSA)-Université de Lyon-Institut National des Sciences Appliquées (INSA)-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Centre National de la Recherche Scientifique (CNRS)-Institut National de la Santé et de la Recherche Médicale (INSERM)-Université Jean Monnet [Saint-Étienne] (UJM)-Hospices Civils de Lyon (HCL)-Institut National des Sciences Appliquées de Lyon (INSA Lyon), Université de Lyon-Centre National de la Recherche Scientifique (CNRS)-Institut National de la Santé et de la Recherche Médicale (INSERM), Indian Institute of Technology Delhi (IIT Delhi), Bayerische Julius-Maximilians University, Tata Institute for Fundamental Research (TIFR), Istituto Nazionale di Fisica Nucleare, Sezione di Firenze (INFN, Sezione di Firenze), Commissariat à l'Energie Atomique, Commissariat à l'énergie atomique et aux énergies alternatives (CEA), University of Glasgow, Institut d'Electronique du Solide et des Systèmes (InESS), Université Louis Pasteur - Strasbourg I-Centre National de la Recherche Scientifique (CNRS), Institute of Microsystems, Vestfold University College, University of Minnesota System, Virgo, Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), Informatics and Telematics Institute/Centre for Research Hellas, Instituto de RadioAstronomía Milimétrica (IRAM), Centre National de la Recherche Scientifique (CNRS), Institut universitaire des systèmes thermiques industriels (IUSTI), Centre National de la Recherche Scientifique (CNRS)-Aix Marseille Université (AMU), Bhabha Atomic Research Centre (BARC), Government of India, Department of Atomic Energy, Université de Bordeaux (UB), Helmholtz zentrum für Schwerionenforschung GmbH (GSI), Univ Turin, Dept Chem, Via P Giuria 7, I-10125 Turin, Italy, Jet Propulsion Laboratory (JPL), NASA-California Institute of Technology (CALTECH), Commissariat à l'énergie atomique et aux énergies alternatives - Laboratoire d'Electronique et de Technologie de l'Information (CEA-LETI), Direction de Recherche Technologique (CEA) (DRT (CEA)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA), Leiden Observatory [Leiden], Universiteit Leiden [Leiden], Centre de Physique des Particules de Marseille (CPPM), Aix Marseille Université (AMU)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Department of Electrical Engineering, University of Pavia, Ecole Superieure de Physique et de Chimie Industrielles de la Ville de Paris (ESPCI Paris), Université Paris sciences et lettres (PSL), European Southern Observatory (ESO), Department of Radiation Oncology, Andrew Love Cancer Centre, Istituto di Fisica dello Spazio Interplanetario (IFSI), Consiglio Nazionale delle Ricerche (CNR), National Research Council of Italy, Research Institute for Hydrological and Geological Hazard Prevention, Department of Physics, Columbia University [New York], Institut de biologie et chimie des protéines [Lyon] (IBCP), Université de Lyon-Université de Lyon-Centre National de la Recherche Scientifique (CNRS), Department of Geological Sciences, University of Michigan [Ann Arbor], University of Michigan System-University of Michigan System, Inter University Accelerator Centre (IUAC), UGC, Photonics and photonic materials group, Departement of Physics, University of bath, University of Bath [Bath], Technical Poultry Manager, Poultry Divisio, Zoetis Brazil, Rothamsted Research, Department of Physics [Roma La Sapienza], Università degli Studi di Roma 'La Sapienza' = Sapienza University [Rome], Friction Stir Laboratory, Brigham Young University (BYU), Institut de recherches sur la catalyse et l'environnement de Lyon (IRCELYON), Université de Lyon-Université de Lyon-Institut de Chimie du CNRS (INC)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de rhéologie (LR), Centre National de la Recherche Scientifique (CNRS)-Institut National Polytechnique de Grenoble (INPG)-Université Joseph Fourier - Grenoble 1 (UJF), Laboratoire de Mesures et Modélisation de la Migration des Radionucléides (L3MR), Service d'Etudes du Comportement des Radionucléides (SECR), Département de Physico-Chimie (DPC), CEA-Direction des Energies (ex-Direction de l'Energie Nucléaire) (CEA-DES (ex-DEN)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay-CEA-Direction des Energies (ex-Direction de l'Energie Nucléaire) (CEA-DES (ex-DEN)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay-Département de Physico-Chimie (DPC), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, Department of Biomedical Sciences, Universita degli Studi di Padova, Istituto Nazionale di Fisica Nucleare, Sezione di Catania (INFN), Università degli studi di Catania [Catania], Unité Mixte de Recherche Epidémiologique et de Surveillance Transport Travail Environnement UMRT9002 (UMRESTTE), Institut National de Recherche sur les Transports et leur Sécurité (INRETS)-Institut de Veille Sanitaire (INVS)-Université Claude Bernard Lyon 1 (UCBL), Laboratory of Image Science and Technology [Nanjing] (LIST), Southeast University [Jiangsu]-School of Computer Science and Engineering, Department of Physics [Gainesville] (UF|Physics), University of Florida [Gainesville] (UF), Istituto Matematico, Scuola Normale Superiore, SensorDynamics AG, Institut d'Astrophysique de Paris (IAP), Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Pierre et Marie Curie - Paris 6 (UPMC), Politecnico di Torino = Polytechnic of Turin (Polito), Ecole Polytechnique Fédérale de Lausanne (EPFL), National Institute of Water and Atmospheric Research [Wellington] (NIWA), Physics Department, University of Wisconsin at Milwaukee, University of Wisconsin - Milwaukee, Departements of Chemistry and Biochemistry, Seattle University [Seattle], Institute for Plasma Research [Gandhinagar], Zurich Research Laboratory, IBM Research GmbH, Inconnu, National Botanical Research Institute, University of Oxford [Oxford], Centre d'étude spatiale des rayonnements (CESR), Observatoire Midi-Pyrénées (OMP), Institut de Recherche pour le Développement (IRD)-Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Université Fédérale Toulouse Midi-Pyrénées-Institut de Recherche pour le Développement (IRD)-Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Toulouse III - Paul Sabatier (UT3), Université Fédérale Toulouse Midi-Pyrénées, School of Earth and Atmospheric Sciences [Atlanta], Department of Materials Science and Engineering, Cornell University, USA, Cornell University [New York], Banaras Hindu University [Varanasi] (BHU), Laboratoire d'études en Géophysique et océanographie spatiales (LEGOS), Institut de Recherche pour le Développement (IRD)-Université Toulouse III - Paul Sabatier (UT3), Université Fédérale Toulouse Midi-Pyrénées-Université Fédérale Toulouse Midi-Pyrénées-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire Midi-Pyrénées (OMP), Institut de Recherche pour le Développement (IRD)-Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Université Fédérale Toulouse Midi-Pyrénées-Institut de Recherche pour le Développement (IRD)-Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Centre National de la Recherche Scientifique (CNRS), The McDonnell Genome Institute (MGI), Washington University in Saint Louis (WUSTL), Laboratoire de Physique des Lasers, Atomes et Molécules - UMR 8523 (PhLAM), Université de Lille-Centre National de la Recherche Scientifique (CNRS), Laboratoire d'études spatiales et d'instrumentation en astrophysique (LESIA), Centre National de la Recherche Scientifique (CNRS)-Université Paris Diderot - Paris 7 (UPD7)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Pierre et Marie Curie - Paris 6 (UPMC), Sezione di Perugia, National High Magnetic Field Laboratory (NHMFL), Florida State University [Tallahassee] (FSU), Key Lab of Computer System and Architecture, Institute of Computing Technology [Beijing] (ICT), Chinese Academy of Sciences [Beijing] (CAS), Centre for Ultrahigh Bandwidth Devices for Optical Systems (CUDOS), Macquarie University, Centre de Recherche en Transplantation et Immunologie (U1064 Inserm - CRTI), Institut National de la Santé et de la Recherche Médicale (INSERM)-Université de Nantes - UFR de Médecine et des Techniques Médicales (UFR MEDECINE), Université de Nantes (UN)-Université de Nantes (UN), Laboratoire de Tribologie et Dynamique des Systèmes (LTDS), École Centrale de Lyon (ECL), Université de Lyon-Université de Lyon-École Nationale des Travaux Publics de l'État (ENTPE)-Ecole Nationale d'Ingénieurs de Saint Etienne-Centre National de la Recherche Scientifique (CNRS), Laboratori Nazionali di Legnaro (LNL), Department of Physiology, Virginia Commonwealth University (VCU)-Medical College of Virginia, Laboratoire Réactions et Génie des Procédés (LRGP), Centre National de la Recherche Scientifique (CNRS)-Université de Lorraine (UL), AIR (AIR), Université de Lyon-Université de Lyon-Institut de Chimie du CNRS (INC)-Centre National de la Recherche Scientifique (CNRS)-Université Claude Bernard Lyon 1 (UCBL), National Astronomical Observatories [Beijing] (NAOC), Université Fédérale Toulouse Midi-Pyrénées-Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS)-Institut de Chimie de Toulouse (ICT-FR 2599), Université Fédérale Toulouse Midi-Pyrénées-Université Fédérale Toulouse Midi-Pyrénées-Institut de Recherche pour le Développement (IRD)-Université Toulouse III - Paul Sabatier (UT3), Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS)-Institut National Polytechnique (Toulouse) (Toulouse INP), Université Fédérale Toulouse Midi-Pyrénées-Institut de Recherche pour le Développement (IRD)-Centre National de la Recherche Scientifique (CNRS), Laboratoire d'Annecy de Physique des Particules (LAPP/Laboratoire d'Annecy-le-Vieux de Physique des Particules), Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7), PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Physique Corpusculaire et Cosmologie - Collège de France (PCC), Collège de France (CdF)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Collège de France (CdF)-Centre National de la Recherche Scientifique (CNRS), Collège de France (CdF)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Université Côte d'Azur (UCA)-Université Côte d'Azur (UCA)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de la Côte d'Azur, Université Côte d'Azur (UCA)-Centre National de la Recherche Scientifique (CNRS), Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Centre National de la Recherche Scientifique (CNRS), Centre National de la Recherche Scientifique (CNRS)-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Institut National des Sciences Appliquées (INSA)-Institut National des Sciences Appliquées (INSA), Centre National de la Recherche Scientifique (CNRS)-École normale supérieure - Paris (ENS Paris)-Centre National de la Recherche Scientifique (CNRS)-École normale supérieure - Paris (ENS Paris)-Collège de France (CdF)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Université de Strasbourg (UNISTRA)-Centre National de la Recherche Scientifique (CNRS)-Matériaux et nanosciences d'Alsace, Université de Strasbourg (UNISTRA)-Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-Institut National de la Santé et de la Recherche Médicale (INSERM)-Centre National de la Recherche Scientifique (CNRS)-Université de Strasbourg (UNISTRA)-Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-Institut National de la Santé et de la Recherche Médicale (INSERM)-Centre National de la Recherche Scientifique (CNRS)-Réseau nanophotonique et optique, Université de Strasbourg (UNISTRA)-Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-Centre National de la Recherche Scientifique (CNRS)-Université de Strasbourg (UNISTRA), Institut für theoretische Physik, Universität Hamburg (UHH)-Universität Hamburg (UHH)-AstroParticule et Cosmologie (APC (UMR_7164)), Met Office Hadley Centre (MOHC), Centre National de la Recherche Scientifique (CNRS)-École normale supérieure - Paris (ENS Paris)-Centre National de la Recherche Scientifique (CNRS)-École normale supérieure - Paris (ENS Paris)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Centre de Recherche Saint-Antoine (CR Saint-Antoine), Institut National de la Santé et de la Recherche Médicale (INSERM)-Université Pierre et Marie Curie - Paris 6 (UPMC), Albert-Einstein-Institut, Max-Planck-Institut, National Institute for Nuclear Physics (INFN), Université de Franche-Comté (UFC)-Centre National de la Recherche Scientifique (CNRS)-Ecole Nationale Supérieure de Mécanique et des Microtechniques (ENSMM)-Université de Technologie de Belfort-Montbeliard (UTBM), Ecosystèmes forestiers (UR EFNO), Institut national de recherche en sciences et technologies pour l'environnement et l'agriculture (IRSTEA), Tata Institute of Fundamental Research [Bombay] (TIFR), University of Minnesota, University of Minnesota [Twin Cities], University of Minnesota System-University of Minnesota System, Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Bhabha Atomic Research Center (BARC), Laboratoire d'Electronique et des Technologies de l'Information (CEA-LETI), Université Grenoble Alpes (UGA)-Direction de Recherche Technologique (CEA) (DRT (CEA)), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Aix Marseille Université (AMU), ESPCI ParisTech, Institute of Climate System, Chinese Academy of Meteorological Sciences (CAMS), Università degli Studi di Roma 'La Sapienza' [Rome], Université Joseph Fourier - Grenoble 1 (UJF)-Institut National Polytechnique de Grenoble (INPG)-Centre National de la Recherche Scientifique (CNRS), CEA-Direction de l'Energie Nucléaire (CEA-DEN), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay-CEA-Direction de l'Energie Nucléaire (CEA-DEN), Université de Lyon-Université de Lyon-Institut National de Recherche sur les Transports et leur Sécurité (INRETS)-Institut de Veille Sanitaire (INVS), Physics Department, University of Florida [Gainesville], Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Politecnico di Torino [Torino] (Polito), University of Wisconsin at Milwaukee, MN2S, Université de Franche-Comté (UFC)-Centre National de la Recherche Scientifique (CNRS)-Ecole Nationale Supérieure de Mécanique et des Microtechniques (ENSMM)-Université de Technologie de Belfort-Montbeliard (UTBM)-Université de Franche-Comté (UFC)-Centre National de la Recherche Scientifique (CNRS)-Ecole Nationale Supérieure de Mécanique et des Microtechniques (ENSMM)-Université de Technologie de Belfort-Montbeliard (UTBM), Institute for Plasma Research, Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS), Cornell University, Université Fédérale Toulouse Midi-Pyrénées-Université Fédérale Toulouse Midi-Pyrénées-Centre National d'Études Spatiales [Toulouse] (CNES)-Observatoire Midi-Pyrénées (OMP), Washington University in St Louis, PSL Research University (PSL)-PSL Research University (PSL)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Pierre et Marie Curie - Paris 6 (UPMC), Laboratoire Matériaux Optiques, Photonique et Systèmes (LMOPS), CentraleSupélec-Université de Lorraine (UL), Université de Lorraine (UL)-Centre National de la Recherche Scientifique (CNRS), Université de Lyon-Université de Lyon-Centre National de la Recherche Scientifique (CNRS)-Université Claude Bernard Lyon 1 (UCBL), Centre National de la Recherche Scientifique (CNRS)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Collège de France (CdF)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Collège de France (CdF)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-AstroParticule et Cosmologie (APC (UMR_7164)), PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Centre National de la Recherche Scientifique (CNRS), PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Institut für theoretische Physik, Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Grenoble Alpes (UGA), Institut de Chimie de Toulouse (ICT), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut de Chimie du CNRS (INC)-Centre National de la Recherche Scientifique (CNRS)-Institut National Polytechnique (Toulouse) (Toulouse INP), Université de Toulouse (UT)-Institut de Recherche pour le Développement (IRD)-Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Centre National de la Recherche Scientifique (CNRS), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Les instituts techniques agricoles (Acta), Radboud University [Nijmegen]-Radboud University [Nijmegen], Université Nice Sophia Antipolis (1965 - 2019) (UNS), COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-Université Côte d'Azur (UCA)-Centre National de la Recherche Scientifique (CNRS), Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), École normale supérieure - Paris (ENS-PSL), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-École normale supérieure - Paris (ENS-PSL), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Collège de France (CdF (institution))-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Université de Strasbourg (UNISTRA)-Institut de Chimie du CNRS (INC)-Centre National de la Recherche Scientifique (CNRS)-Matériaux et Nanosciences Grand-Est (MNGE), Université de Strasbourg (UNISTRA)-Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-Institut National de la Santé et de la Recherche Médicale (INSERM)-Institut de Chimie du CNRS (INC)-Centre National de la Recherche Scientifique (CNRS)-Université de Strasbourg (UNISTRA)-Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-Institut National de la Santé et de la Recherche Médicale (INSERM)-Centre National de la Recherche Scientifique (CNRS)-Réseau nanophotonique et optique, Université de Strasbourg (UNISTRA)-Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-Centre National de la Recherche Scientifique (CNRS)-Université de Strasbourg (UNISTRA)-Centre National de la Recherche Scientifique (CNRS), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut für theoretische Physik, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), University of Naples Federico II = Università degli studi di Napoli Federico II, Leibniz Universität Hannover=Leibniz University Hannover, Université de Technologie de Belfort-Montbeliard (UTBM)-Ecole Nationale Supérieure de Mécanique et des Microtechniques (ENSMM)-Centre National de la Recherche Scientifique (CNRS)-Université de Franche-Comté (UFC), Université Bourgogne Franche-Comté [COMUE] (UBFC)-Université Bourgogne Franche-Comté [COMUE] (UBFC), Université de Lyon-Institut National des Sciences Appliquées (INSA)-Institut National des Sciences Appliquées (INSA)-Université Jean Monnet - Saint-Étienne (UJM)-Institut National de la Santé et de la Recherche Médicale (INSERM)-Centre National de la Recherche Scientifique (CNRS)-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Institut National des Sciences Appliquées (INSA)-Institut National des Sciences Appliquées (INSA)-Université Jean Monnet - Saint-Étienne (UJM)-Institut National de la Santé et de la Recherche Médicale (INSERM)-Centre National de la Recherche Scientifique (CNRS), Aix Marseille Université (AMU)-Centre National de la Recherche Scientifique (CNRS), Universiteit Leiden, Università degli Studi di Pavia = University of Pavia (UNIPV), National Research Council of Italy | Consiglio Nazionale delle Ricerche (CNR), Biotechnology and Biological Sciences Research Council (BBSRC), Dipartimento di Fisica [Roma La Sapienza], Università degli Studi di Roma 'La Sapienza' = Sapienza University [Rome] (UNIROMA), Università degli Studi di Padova = University of Padua (Unipd), Università degli studi di Catania = University of Catania (Unict), Scuola Normale Superiore di Pisa (SNS), University of Oxford, Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire Midi-Pyrénées (OMP), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Institut de Recherche pour le Développement (IRD)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Centre National de la Recherche Scientifique (CNRS), Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université de Lyon-Université de Lyon-École Nationale des Travaux Publics de l'État (ENTPE)-Ecole Nationale d'Ingénieurs de Saint Etienne (ENISE)-Centre National de la Recherche Scientifique (CNRS), Massachusetts Institute of Technology. Department of Physics, Lincoln Laboratory, MIT Kavli Institute for Astrophysics and Space Research, CALTECH, Louisiana State Univ, Amer Univ, Univ Salerno, INFN, Univ Florida, LIGO Livingston Observ, Univ Savoie Mont Blanc, Univ Sannio Benevento, Max Planck Inst Gravitat Phys, Nikhef, MIT, Inst Nacl Pesquisas Espaciais, Inter Univ Ctr Astron & Astrophys, Tata Inst Fundamental Res, Univ Wisconsin, Leibniz Univ Hannover, Univ Pisa, Australian Natl Univ, Calif State Univ Fullerton, Univ Paris 11, Chennai Math Inst, Univ Roma Tor Vergata, Univ Hamburg, Universidade de São Paulo (USP), West Virginia Univ, Univ Perugia, EGO, Syracuse Univ, Univ Glasgow, LIGO Hanford Observ, Wigner RCP, Columbia Univ, Stanford Univ, Univ Padua, Polish Acad Sci, Georgia Inst Technol, Univ Birmingham, Univ Genoa, RRCAT, Lomonosov Moscow State Univ, Univ West Scotland, Caltech CaRT, Univ Western Australia, Radboud Univ Nijmegen, Univ Cote dAzur, Univ Rennes 1, Washington State Univ, Univ Urbino Carlo Bo, Univ Oregon, UPMC Sorbonne Univ, Carleton Coll, Astron Observ Warsaw Univ, Vrije Univ Amsterdam, Univ Maryland, CNRS, Univ Claude Bernard Lyon 1, Univ Napoli Federico II, NASA, Univ Tokyo, Univ Adelaide, Tsinghua Univ, Texas Tech Univ, Univ Mississippi, Penn State Univ, Natl Tsing Hua Univ, Charles Sturt Univ, Univ Chicago, Kenyon Coll, Korea Inst Sci & Technol Informat, Univ Cambridge, Univ Roma La Sapienza, Univ Libre Bruxelles, Sonoma State Univ, Montana State Univ, Northwestern Univ, Univ Illes Balears, Univ Texas Rio Grande Valley, Bellevue Coll, Inst Plasma Res, Univ Sheffield, Calif State Univ Los Angeles, Univ Trento, Cardiff Univ, Montclair State Univ, Natl Astron Observ Japan, Univ Toronto, MTA Eotvos Univ, Univ Edinburgh, Univ & Inst Adv Res, IISER TVM, Univ Szeged, Embry Riddle Aeronaut Univ, INAF, Univ Michigan, Rochester Inst Technol, Univ Illinois, Univ Bialystok, Univ Strathclyde, Univ Southampton, Univ Washington Bothell, Inst Appl Phys, Seoul Natl Univ, Inje Univ Gimhae, Natl Inst Math Sci, Pusan Natl Univ, NCBJ, Monash Univ, Hanyang Univ, Chinese Univ Hong Kong, Univ Alabama Huntsville, Univ Minnesota, Univ Camerino, Southern Univ & A&M Coll, Univ Melbourne, Coll William & Mary, Universidade Estadual Paulista (Unesp), Whitman Coll, Univ Lyon, Hobart & William Smith Colleges, Univ Zielona Gora, Univ London, IISER Kolkata, Indian Inst Technol, Andrews Univ, Univ Siena, Trinity Univ, Univ Washington, Abilene Christian Univ, (Astro)-Particles Physics, Abbott, B. P., Abbott, R., Abbott, T. D., Abernathy, M. R., Acernese, F., Ackley, K., Adams, C., Adams, T., Addesso, P., Adhikari, R. X., Adya, V. B., Affeldt, C., Agathos, M., Agatsuma, K., Aggarwal, N., Aguiar, O. D., Aiello, L., Ain, A., Ajith, P., Allen, B., Allocca, A., Altin, P. A., Ananyeva, A., Anderson, S. B., Anderson, W. G., Appert, S., Arai, K., Araya, M. C., Areeda, J. S., Arnaud, N., Arun, K. G., Ascenzi, S., Ashton, G., Ast, M., Aston, S. M., Astone, P., Aufmuth, P., Aulbert, C., Avila-Alvarez, A., Babak, S., Bacon, P., Bader, M. K. M., Baker, P. T., Baldaccini, F., Ballardin, G., Ballmer, S. W., Barayoga, J. C., Barclay, S. E., Barish, B. C., Barker, D., Barone, F., Barr, B., Barsotti, L., Barsuglia, M., Barta, D., Bartlett, J., Bartos, I., Bassiri, R., Basti, A., Batch, J. C., Baune, C., Bavigadda, V., Bazzan, M., Beer, C., Bejger, M., Belahcene, I., Belgin, M., Bell, A. S., Berger, B. K., Bergmann, G., Berry, C. P. L., Bersanetti, D., Bertolini, A., Betzwieser, J., Bhagwat, S., Bhandare, R., Bilenko, I. A., Billingsley, G., Billman, C. R., Birch, J., Birney, R., Birnholtz, O., Biscans, S., Bisht, A., Bitossi, M., Biwer, C., Bizouard, M. A., Blackburn, J. K., Blackman, J., Blair, C. D., Blair, D. G., Blair, R. M., Bloemen, S., Bock, O., Boer, M., Bogaert, G., Bohe, A., Bondu, F., Bonnand, R., Boom, B. A., Bork, R., Boschi, V., Bose, S., Bouffanais, Y., Bozzi, A., Bradaschia, C., Brady, P. R., Braginsky, V. B., Branchesi, M., Brau, J. E., Briant, T., Brillet, A., Brinkmann, M., Brisson, V., Brockill, P., Broida, J. E., Brooks, A. F., Brown, D. A., Brown, D. D., Brown, N. M., Brunett, S., Buchanan, C. C., Buikema, A., Bulik, T., Bulten, H. J., Buonanno, A., Buskulic, D., Buy, C., Byer, R. L., Cabero, M., Cadonati, L., Cagnoli, G., Cahillane, C., Calderón Bustillo, J., Callister, T. A., Calloni, E., Camp, J. B., Canepa, M., Cannon, K. C., Cao, H., Cao, J., Capano, C. D., Capocasa, E., Carbognani, F., Caride, S., Casanueva Diaz, J., Casentini, C., Caudill, S., Cavaglià, M., Cavalier, F., Cavalieri, R., Cella, G., Cepeda, C. B., Cerboni Baiardi, L., Cerretani, G., Cesarini, E., Chamberlin, S. J., Chan, M., Chao, S., Charlton, P., Chassande-Mottin, E., Cheeseboro, B. D., Chen, H. Y., Chen, Y., Cheng, H. -P., Chincarini, A., Chiummo, A., Chmiel, T., Cho, H. S., Cho, M., Chow, J. H., Christensen, N., Chu, Q., Chua, A. J. K., Chua, S., Chung, S., Ciani, G., Clara, F., Clark, J. A., Cleva, F., Cocchieri, C., Coccia, E., Cohadon, P. -F., Colla, A., Collette, C. G., Cominsky, L., Constancio, M., Conti, L., Cooper, S. J., Corbitt, T. R., Cornish, N., Corsi, A., Cortese, S., Costa, C. A., Coughlin, M. W., Coughlin, S. B., Coulon, J. -P., Countryman, S. T., Couvares, P., Covas, P. B., Cowan, E. E., Coward, D. M., Cowart, M. J., Coyne, D. C., Coyne, R., Creighton, J. D. E., Creighton, T. D., Cripe, J., Crowder, S. G., Cullen, T. J., Cumming, A., Cunningham, L., Cuoco, E., Dal Canton, T., Danilishin, S. L., D'Antonio, S., Danzmann, K., Dasgupta, A., Da Silva Costa, C. F., Dattilo, V., Dave, I., Davier, M., Davies, G. S., Davis, D., Daw, E. J., Day, B., Day, R., De, S., Debra, D., Debreczeni, G., Degallaix, J., De Laurentis, M., Deléglise, S., Del Pozzo, W., Denker, T., Dent, T., Dergachev, V., De Rosa, Rosario., Derosa, R. T., Desalvo, R., Devine, R. C., Dhurandhar, S., Díaz, M. C., Di Fiore, L., Di Giovanni, M., Di Girolamo, T., Di Lieto, A., Di Pace, S., Di Palma, I., Di Virgilio, A., Doctor, Z., Dolique, V., Donovan, F., Dooley, K. L., Doravari, S., Dorrington, I., Douglas, R., Dovale Álvarez, M., Downes, T. P., Drago, M., Drever, R. W. P., Driggers, J. C., Du, Z., Ducrot, M., Dwyer, S. E., Edo, T. B., Edwards, M. C., Effler, A., Eggenstein, H. -B., Ehrens, P., Eichholz, J., Eikenberry, S. S., Eisenstein, R. A., Essick, R. C., Etienne, Z., Etzel, T., Evans, M., Evans, T. M., Everett, R., Factourovich, M., Fafone, V., Fair, H., Fairhurst, S., Fan, X., Farinon, S., Farr, B., Farr, W. M., Fauchon-Jones, E. J., Favata, M., Fays, M., Fehrmann, H., Fejer, M. M., Fernández Galiana, A., Ferrante, I., Ferreira, E. C., Ferrini, F., Fidecaro, F., Fiori, I., Fiorucci, D., Fisher, R. P., Flaminio, R., Fletcher, M., Fong, H., Forsyth, S. S., Fournier, J. -D., Frasca, S., Frasconi, F., Frei, Z., Freise, A., Frey, R., Frey, V., Fries, E. M., Fritschel, P., Frolov, V. V., Fulda, P., Fyffe, M., Gabbard, H., Gadre, B. U., Gaebel, S. M., Gair, J. R., Gammaitoni, L., Gaonkar, S. G., Garufi, F., Gaur, G., Gayathri, V., Gehrels, N., Gemme, G., Genin, E., Gennai, A., George, J., Gergely, L., Germain, V., Ghonge, S., Ghosh, Abhirup, Ghosh, Archisman, Ghosh, S., Giaime, J. A., Giardina, K. D., Giazotto, A., Gill, K., Glaefke, A., Goetz, E., Goetz, R., Gondan, L., González, G., Gonzalez Castro, J. M., Gopakumar, A., Gorodetsky, M. L., Gossan, S. E., Gosselin, M., Gouaty, R., Grado, A., Graef, C., Granata, M., Grant, A., Gras, S., Gray, C., Greco, G., Green, A. C., Groot, P., Grote, H., Grunewald, S., Guidi, G. M., Guo, X., Gupta, A., Gupta, M. K., Gushwa, K. E., Gustafson, E. K., Gustafson, R., Hacker, J. J., Hall, B. R., Hall, E. D., Hammond, G., Haney, M., Hanke, M. M., Hanks, J., Hanna, C., Hanson, J., Hardwick, T., Harms, J., Harry, G. M., Harry, I. W., Hart, M. J., Hartman, M. T., Haster, C. -J., Haughian, K., Healy, J., Heidmann, A., Heintze, M. C., Heitmann, H., Hello, P., Hemming, G., Hendry, M., Heng, I. S., Hennig, J., Henry, J., Heptonstall, A. W., Heurs, M., Hild, S., Hoak, D., Hofman, D., Holt, K., Holz, D. E., Hopkins, P., Hough, J., Houston, E. A., Howell, E. J., Hu, Y. M., Huerta, E. A., Huet, D., Hughey, B., Husa, S., Huttner, S. H., Huynh-Dinh, T., Indik, N., Ingram, D. R., Inta, R., Isa, H. N., Isac, J. -M., Isi, M., Isogai, T., Iyer, B. R., Izumi, K., Jacqmin, T., Jani, K., Jaranowski, P., Jawahar, S., Jiménez-Forteza, F., Johnson, W. W., Jones, D. I., Jones, R., Jonker, R. J. G., Ju, L., Junker, J., Kalaghatgi, C. V., Kalogera, V., Kandhasamy, S., Kang, G., Kanner, J. B., Karki, S., Karvinen, K. S., Kasprzack, M., Katsavounidis, E., Katzman, W., Kaufer, S., Kaur, T., Kawabe, K., Kéfélian, F., Keitel, D., Kelley, D. B., Kennedy, R., Key, J. S., Khalili, F. Y., Khan, I., Khan, S., Khan, Z., Khazanov, E. A., Kijbunchoo, N., Kim, Chunglee, Kim, J. C., Kim, Whansun, Kim, W., Kim, Y. -M., Kimbrell, S. J., King, E. J., King, P. J., Kirchhoff, R., Kissel, J. S., Klein, B., Kleybolte, L., Klimenko, S., Koch, P., Koehlenbeck, S. M., Koley, S., Kondrashov, V., Kontos, A., Korobko, M., Korth, W. Z., Kowalska, I., Kozak, D. B., Krämer, C., Kringel, V., Krishnan, B., Królak, A., Kuehn, G., Kumar, P., Kumar, R., Kuo, L., Kutynia, A., Lackey, B. D., Landry, M., Lang, R. N., Lange, J., Lantz, B., Lanza, R. K., Lartaux-Vollard, A., Lasky, P. D., Laxen, M., Lazzarini, A., Lazzaro, C., Leaci, P., Leavey, S., Lebigot, E. O., Lee, C. H., Lee, H. K., Lee, H. M., Lee, K., Lehmann, J., Lenon, A., Leonardi, M., Leong, J. R., Leroy, N., Letendre, N., Levin, Y., Li, T. G. F., Libson, A., Littenberg, T. B., Liu, J., Lockerbie, N. A., Lombardi, A. L., London, L. T., Lord, J. E., Lorenzini, M., Loriette, V., Lormand, M., Losurdo, G., Lough, J. D., Lovelace, G., Lück, H., Lundgren, A. P., Lynch, R., Ma, Y., Macfoy, S., Machenschalk, B., Macinnis, M., Macleod, D. M., Magaña-Sandoval, F., Majorana, E., Maksimovic, I., Malvezzi, V., Man, N., Mandic, V., Mangano, V., Mansell, G. L., Manske, M., Mantovani, M., Marchesoni, F., Marion, F., Márka, S., Márka, Z., Markosyan, A. S., Maros, E., Martelli, F., Martellini, L., Martin, I. W., Martynov, D. V., Mason, K., Masserot, A., Massinger, T. J., Masso-Reid, M., Mastrogiovanni, S., Matichard, F., Matone, L., Mavalvala, N., Mazumder, N., Mccarthy, R., Mcclelland, D. E., Mccormick, S., Mcgrath, C., Mcguire, S. C., Mcintyre, G., Mciver, J., Mcmanus, D. J., Mcrae, T., Mcwilliams, S. T., Meacher, D., Meadors, G. D., Meidam, J., Melatos, A., Mendell, G., Mendoza-Gandara, D., Mercer, R. A., Merilh, E. L., Merzougui, M., Meshkov, S., Messenger, C., Messick, C., Metzdorff, R., Meyers, P. M., Mezzani, F., Miao, H., Michel, C., Middleton, H., Mikhailov, E. E., Milano, L., Miller, A. L., Miller, A., Miller, B. B., Miller, J., Millhouse, M., Minenkov, Y., Ming, J., Mirshekari, S., Mishra, C., Mitra, S., Mitrofanov, V. P., Mitselmakher, G., Mittleman, R., Moggi, A., Mohan, M., Mohapatra, S. R. P., Montani, M., Moore, B. C., Moore, C. J., Moraru, D., Moreno, G., Morriss, S. R., Mours, B., Mow-Lowry, C. M., Mueller, G., Muir, A. W., Mukherjee, Arunava, Mukherjee, D., Mukherjee, S., Mukund, N., Mullavey, A., Munch, J., Muniz, E. A. M., Murray, P. G., Mytidis, A., Napier, K., Nardecchia, I., Naticchioni, L., Nelemans, G., Nelson, T. J. N., Neri, M., Nery, M., Neunzert, A., Newport, J. M., Newton, G., Nguyen, T. T., Nielsen, A. B., Nissanke, S., Nitz, A., Noack, A., Nocera, F., Nolting, D., Normandin, M. E. N., Nuttall, L. K., Oberling, J., Ochsner, E., Oelker, E., Ogin, G. H., Oh, J. J., Oh, S. H., Ohme, F., Oliver, M., Oppermann, P., Oram, Richard J, O'Reilly, B., O'Shaughnessy, R., Ottaway, D. J., Overmier, H., Owen, B. J., Pace, A. E., Page, J., Pai, A., Pai, S. A., Palamos, J. R., Palashov, O., Palomba, C., Pal-Singh, A., Pan, H., Pankow, C., Pannarale, F., Pant, B. C., Paoletti, F., Paoli, A., Papa, M. A., Paris, H. R., Parker, W., Pascucci, D., Pasqualetti, A., Passaquieti, R., Passuello, D., Patricelli, B., Pearlstone, B. L., Pedraza, M., Pedurand, R., Pekowsky, L., Pele, A., Penn, S., Perez, C. J., Perreca, A., Perri, L. M., Pfeiffer, H. P., Phelps, M., Piccinni, O. J., Pichot, M., Piergiovanni, F., Pierro, V., Pillant, G., Pinard, L., Pinto, I. M., Pitkin, M., Poe, M., Poggiani, R., Popolizio, P., Post, A., Powell, J., Prasad, J., Pratt, J. W. W., Predoi, V., Prestegard, T., Prijatelj, M., Principe, M., Privitera, S., Prix, R., Prodi, G. A., Prokhorov, L. G., Puncken, O., Punturo, M., Puppo, P., Pürrer, M., Qi, H., Qin, J., Qiu, S., Quetschke, V., Quintero, E. A., Quitzow-James, R., Raab, F. J., Rabeling, D. S., Radkins, H., Raffai, P., Raja, S., Rajan, C., Rakhmanov, M., Rapagnani, P., Raymond, V., Razzano, M., Re, V., Read, J., Regimbau, T., Rei, L., Reid, S., Reitze, D. H., Rew, H., Reyes, S. D., Rhoades, E., Ricci, F., Riles, K., Rizzo, M., Robertson, N. A., Robie, R., Robinet, F., Rocchi, A., Rolland, L., Rollins, J. G., Roma, V. J., Romano, J. D., Romano, R., Romie, J. H., Rosińska, D., Rowan, S., Rüdiger, A., Ruggi, P., Ryan, K., Sachdev, S., Sadecki, T., Sadeghian, L., Sakellariadou, M., Salconi, L., Saleem, M., Salemi, F., Samajdar, A., Sammut, L., Sampson, L. M., Sanchez, E. J., Sandberg, V., Sanders, J. R., Sassolas, B., Saulson, P. R., Sauter, O., Savage, R. L., Sawadsky, A., Schale, P., Scheuer, J., Schmidt, E., Schmidt, J., Schmidt, P., Schnabel, R., Schofield, R. M. S., Schönbeck, A., Schreiber, E., Schuette, D., Schutz, B. F., Schwalbe, S. G., Scott, J., Scott, S. M., Sellers, D., Sengupta, A. S., Sentenac, D., Sequino, V., Sergeev, A., Setyawati, Y., Shaddock, D. A., Shaffer, T. J., Shahriar, M. S., Shapiro, B., Shawhan, P., Sheperd, A., Shoemaker, D. H., Shoemaker, D. M., Siellez, K., Siemens, X., Sieniawska, M., Sigg, D., Silva, A. D., Singer, A., Singer, L. P., Singh, A., Singh, R., Singhal, A., Sintes, A. M., Slagmolen, B. J. J., Smith, B., Smith, J. R., Smith, R. J. E., Son, E. J., Sorazu, B., Sorrentino, F., Souradeep, T., Spencer, A. P., Srivastava, A. K., Staley, A., Steinke, M., Steinlechner, J., Steinlechner, S., Steinmeyer, D., Stephens, B. C., Stevenson, S. P., Stone, R., Strain, K. A., Straniero, N., Stratta, G., Strigin, S. E., Sturani, R., Stuver, A. L., Summerscales, T. Z., Sun, L., Sunil, S., Sutton, P. J., Swinkels, B. L., Szczepańczyk, M. J., Tacca, M., Talukder, D., Tanner, D. B., Tápai, M., Taracchini, A., Taylor, R., Theeg, T., Thomas, E. G., Thomas, M., Thomas, P., Thorne, K. A., Thrane, E., Tippens, T., Tiwari, S., Tiwari, V., Tokmakov, K. V., Toland, K., Tomlinson, C., Tonelli, M., Tornasi, Z., Torrie, C. I., Töyrä, D., Travasso, F., Traylor, G., Trifirò, D., Trinastic, J., Tringali, M. C., Trozzo, L., Tse, M., Tso, R., Turconi, M., Tuyenbayev, D., Ugolini, D., Unnikrishnan, C. S., Urban, A. L., Usman, S. A., Vahlbruch, H., Vajente, G., Valdes, G., Van Bakel, N., Van Beuzekom, M., Van Den Brand, J. F. J., Van Den Broeck, C., Vander-Hyde, D. C., Van Der Schaaf, L., Van Heijningen, J. V., Van Veggel, A. A., Vardaro, M., Varma, V., Vass, S., Vasúth, M., Vecchio, A., Vedovato, G., Veitch, J., Veitch, P. J., Venkateswara, K., Venugopalan, G., Verkindt, D., Vetrano, F., Viceré, A., Viets, A. D., Vinciguerra, S., Vine, D. J., Vinet, J. -Y., Vitale, S., Vo, T., Vocca, H., Vorvick, C., Voss, D. V., Vousden, W. D., Vyatchanin, S. P., Wade, A. R., Wade, L. E., Wade, M., Walker, M., Wallace, L., Walsh, S., Wang, G., Wang, H., Wang, M., Wang, Y., Ward, R. L., Warner, J., Was, M., Watchi, J., Weaver, B., Wei, L. -W., Weinert, M., Weinstein, A. J., Weiss, R., Wen, L., Weßels, P., Westphal, T., Wette, K., Whelan, J. T., Whiting, B. F., Whittle, C., Williams, D., Williams, R. D., Williamson, A. R., Willis, J. L., Willke, B., Wimmer, M. H., Winkler, W., Wipf, C. C., Wittel, H., Woan, G., Woehler, J., Worden, J., Wright, J. L., Wu, D. S., Wu, G., Yam, W., Yamamoto, H., Yancey, C. C., Yap, M. J., Yu, Hang, Yu, Haocun, Yvert, M., Zadrożny, A., Zangrando, L., Zanolin, M., Zendri, J. -P., Zevin, M., Zhang, L., Zhang, M., Zhang, T., Zhang, Y., Zhao, C., Zhou, M., Zhou, Z., Zhu, S. J., Zhu, X. J., Zucker, M. E., and Zweizig, J.
Subjects: Physics and Astronomy (miscellaneous), Astrophysics::High Energy Astrophysical Phenomena, Astronomy, FOS: Physical sciences, General Relativity and Quantum Cosmology (gr-qc), Astrophysics, LIGO-Virgo, Magnetar, 01 natural sciences, General Relativity and Quantum Cosmology, Gravitational waves, long transients, LIGO, Gravitational waves, UPPER LIMITS, Search algorithm, SIGNALS, 0103 physical sciences, Waveform, long transients, High Energy Physics, LIGO, 010306 general physics, gravitational wave, 010303 astronomy & astrophysics, ComputingMilieux_MISCELLANEOUS, QC, QB, High Energy Astrophysical Phenomena (astro-ph.HE), Physics, gravitational waves, long duration transient, [PHYS]Physics [physics], Gravitational wave, Black hole, MODEL, Neutron star, Amplitude, BLACK-HOLE, ComputingMethodologies_DOCUMENTANDTEXTPROCESSING, RADIATION, NEUTRINO, Astrophysics - High Energy Astrophysical Phenomena, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
Abstract: Made available in DSpace on 2018-11-26T17:45:14Z (GMT). No. of bitstreams: 0 Previous issue date: 2018-03-22 Australian Research Council Council of Scientific and Industrial Research of India Department of Science and Technology, India Science AMP; Engineering Research Board (SERB), India Ministry of Human Resource Development, India Spanish Agencia Estatal de Investigacion Vicepresidencia i Conselleria d'Innovacio, Recerca i Turisme Conselleria d'Educacio i Universitat del Govern de les Illes Balears Conselleria d'Educacio, Investigacio, Cultura i Esport de la Generalitat Valenciana National Science Centre of Poland Swiss National Science Foundation (SNSF) Russian Foundation for Basic Research Russian Science Foundation European Commission European Regional Development Funds (ERDF) Royal Society Scottish Funding Council Scottish Universities Physics Alliance Hungarian Scientific Research Fund (OTKA) Lyon Institute of Origins (LIO) Paris Ile-de-France Region National Research, Development and Innovation Office Hungary (NKFI) National Research Foundation of Korea Industry Canada Province of Ontario through the Ministry of Economic Development and Innovation Natural Science and Engineering Research Council Canada Canadian Institute for Advanced Research Brazilian Ministry of Science, Technology, Innovations, and Communications International Center for Theoretical Physics South American Institute for Fundamental Research (ICTP-SAIFR) Research Grants Council of Hong Kong National Natural Science Foundation of China (NSFC) Leverhulme Trust Ministry of Science and Technology (MOST), Taiwan Kavli Foundation EGO consortium We present the results of a search for long-duration gravitational wave transients in the data of the LIGO Hanford and LIGO Livingston second generation detectors between September 2015 and January 2016, with a total observational time of 49 d. The search targets gravitational wave transients of 10-500 s duration in a frequency band of 24-2048 Hz, with minimal assumptions about the signal waveform, polarization, source direction, or time of occurrence. No significant events were observed. As a result we set 90% confidence upper limits on the rate of long-duration gravitational wave transients for different types of gravitational wave signals. We also show that the search is sensitive to sources in the Galaxy emitting at least similar to 10-8 M(circle dot)c(2) in gravitational waves. CALTECH, LIGO, Pasadena, CA 91125 USA Louisiana State Univ, Baton Rouge, LA 70803 USA Amer Univ, Washington, DC 20016 USA Univ Salerno, I-84084 Salerno, Italy INFN, Sez Napoli, Complesso Univ Monte S Angelo, I-80126 Naples, Italy Univ Florida, Gainesville, FL 32611 USA LIGO Livingston Observ, Livingston, LA 70754 USA Univ Savoie Mont Blanc, CNRS, Lab Annecy le Vieux Phys Particules LAPP, IN2P3, F-74941 Annecy Le Vieux, France Univ Sannio Benevento, I-82100 Benevento, Italy Max Planck Inst Gravitat Phys, Albert Einstein Inst, D-30167 Hannover, Germany Nikhef, Sci Pk, NL-1098 XG Amsterdam, Netherlands MIT, LIGO, Cambridge, MA 02139 USA Inst Nacl Pesquisas Espaciais, BR-12227010 Sao Jose Dos Campos, Brazil INFN, Gran Sasso Sci Inst, I-67100 Laquila, Italy INFN, Sez Roma Tor Vergata, I-00133 I- Roma, Italy Inter Univ Ctr Astron & Astrophys, Pune 411007, Maharashtra, India Tata Inst Fundamental Res, Int Ctr Theoret Sci, Bengaluru 560089, India Univ Wisconsin, Milwaukee, WI 53201 USA Leibniz Univ Hannover, D-30167 Hannover, Germany Univ Pisa, I-56127 Pisa, Italy INFN, Sez Pisa, I-56127 Pisa, Italy Australian Natl Univ, Canberra, ACT 0200, Australia Calif State Univ Fullerton, Fullerton, CA 92831 USA Univ Paris 11, Univ Paris Saclay, CNRS IN2P3, LAL, F-91898 Orsay, France Chennai Math Inst, Madras 603103, Tamil Nadu, India Univ Roma Tor Vergata, I-00133 Rome, Italy Univ Hamburg, D-22761 Hamburg, Germany INFN, Sez Roma, I-00185 Rome, Italy Max Planck Inst Gravitat Phys, Albert Einstein Inst, D-14476 Potsdam, Germany Univ Paris Diderot, CNRS IN2P3, Sorbonne Paris Cite, CEA Irfu,APC,Observ Paris,AstroParticule & Cosmol, F-75205 Paris 13, France West Virginia Univ, Morgantown, WV 26506 USA West Virginia Univ, Ctr Gravitat Waves & Cosmol, Morgantown, WV 26505 USA Univ Perugia, I-06123 Perugia, Italy INFN, Sez Perugia, I-06123 Perugia, Italy EGO, I-56021 Pisa, Italy Syracuse Univ, Syracuse, NY 13244 USA Univ Glasgow, SUPA, Glasgow G12 8QQ, Lanark, Scotland LIGO Hanford Observ, Richland, WA 99352 USA Wigner RCP, RMKI, Konkoly Thege Miklos Ut 29-33, H-1121 Budapest, Hungary Columbia Univ, New York, NY 10027 USA Stanford Univ, Stanford, CA 94305 USA Univ Padua, Dipartimento Fis & Astron, I-35131 Padua, Italy INFN, Sez Padova, I-35131 Padua, Italy Polish Acad Sci, Nicolaus Copernicus Astron Ctr, PL-00716 Warsaw, Poland Georgia Inst Technol, Ctr Relativist Astrophys, Atlanta, GA 30332 USA Georgia Inst Technol, Sch Phys, Atlanta, GA 30332 USA Univ Birmingham, Birmingham B15 2TT, W Midlands, England Univ Genoa, I-16146 Genoa, Italy INFN, Sez Genova, I-16146 Genoa, Italy RRCAT, Indore 452013, Madhya Pradesh, India Lomonosov Moscow State Univ, Fac Phys, Moscow 119991, Russia Univ West Scotland, SUPA, Paisley PA1 2BE, Renfrew, Scotland Caltech CaRT, Pasadena, CA 91125 USA Univ Western Australia, Crawley, WA 6009, Australia Radboud Univ Nijmegen, Dept Astrophys IMAPP, POB 9010, NL-6500 GL Nijmegen, Netherlands Univ Cote dAzur, CNRS, Artemis, Observ Cote dAzur, CS 34229, F-06304 Nice 4, France Univ Rennes 1, CNRS, Inst Phys Rennes, F-35042 Rennes, France Washington State Univ, Pullman, WA 99164 USA Univ Urbino Carlo Bo, I-61029 Urbino, Italy INFN, Sez Firenze, I-50019 Florence, Italy Univ Oregon, Eugene, OR 97403 USA UPMC Sorbonne Univ, Coll France, ENS PSL Res Univ, CNRS,Lab Kastler Brossel, F-75005 Paris, France Carleton Coll, Northfield, MN 55057 USA Astron Observ Warsaw Univ, PL-00478 Warsaw, Poland Vrije Univ Amsterdam, NL-1081 HV Amsterdam, Netherlands Univ Maryland, College Pk, MD 20742 USA CNRS, LMA, IN2P3, F-69622 Villeurbanne, France Univ Claude Bernard Lyon 1, F-69622 Villeurbanne, France Univ Napoli Federico II, Complesso Univ Monte S Angelo, I-80126 Naples, Italy NASA, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA Univ Tokyo, RESCEU, Tokyo 1130033, Japan Univ Adelaide, Adelaide, SA 5005, Australia Tsinghua Univ, Beijing 100084, Peoples R China Texas Tech Univ, Lubbock, TX 79409 USA Univ Mississippi, University, MS 38677 USA Penn State Univ, University Pk, PA 16802 USA Natl Tsing Hua Univ, Hsinchu 30013, Taiwan Charles Sturt Univ, Wagga Wagga, NSW 2678, Australia Univ Chicago, Chicago, IL 60637 USA Kenyon Coll, Gambier, OH 43022 USA Korea Inst Sci & Technol Informat, Daejeon 305806, South Korea Univ Cambridge, Cambridge CB2 1TN, England Univ Roma La Sapienza, I-00185 Rome, Italy Univ Libre Bruxelles, B-1050 Brussels, Belgium Sonoma State Univ, Rohnert Pk, CA 94928 USA Montana State Univ, Bozeman, MT 59717 USA Northwestern Univ, CIERA, Evanston, IL 60208 USA Univ Illes Balears, IEEC IAC3, E-07122 Palma De Mallorca, Spain Univ Texas Rio Grande Valley, Brownsville, TX 78520 USA Bellevue Coll, Bellevue, WA 98007 USA Inst Plasma Res, Bhat 382428, Gandhinagar, India Univ Sheffield, Sheffield S10 2TN, S Yorkshire, England Calif State Univ Los Angeles, 5154 State Univ Dr, Los Angeles, CA 90032 USA Univ Trento, Dipartimento Fis, I-38123 Povo, Trento, Italy INFN, Trento Inst Fundamental Phys & Applicat, I-38123 Povo, Trento, Italy Cardiff Univ, Cardiff CF24 3AA, S Glam, Wales Montclair State Univ, Montclair, NJ 07043 USA Natl Astron Observ Japan, 2-21-1 Osawa, Mitaka, Tokyo 1818588, Japan Univ Toronto, Canadian Inst Theoret Astrophys, Toronto, ON M5S 3H8, Canada MTA Eotvos Univ, Lendulet Astrophys Res Grp, H-1117 Budapest, Hungary Univ Edinburgh, Sch Math, Edinburgh EH9 3FD, Midlothian, Scotland Univ & Inst Adv Res, Gandhinagar 382007, Gujarat, India IISER TVM, CET Campus, Trivandrum 695016, Kerala, India Univ Szeged, Dom Ter 9, H-6720 Szeged, Hungary Embry Riddle Aeronaut Univ, Prescott, AZ 86301 USA Tata Inst Fundamental Res, Bombay 400005, Maharashtra, India INAF, Osservatorio Astron Capodimonte, I-80131 Naples, Italy Univ Michigan, Ann Arbor, MI 48109 USA Rochester Inst Technol, Rochester, NY 14623 USA Univ Illinois, NCSA, Urbana, IL 61801 USA Univ Bialystok, PL-15424 Bialystok, Poland Univ Strathclyde, SUPA, Glasgow G1 1XQ, Lanark, Scotland Univ Southampton, Southampton SO17 1BJ, Hants, England Univ Washington Bothell, 18115 Campus Way NE, Bothell, WA 98011 USA Inst Appl Phys, Nizhnii Novgorod 603950, Russia Seoul Natl Univ, Seoul 151742, South Korea Inje Univ Gimhae, South Gyeongsang 621749, South Korea Natl Inst Math Sci, Daejeon 305390, South Korea Pusan Natl Univ, Busan 609735, South Korea NCBJ, PL-05400 Otwock, Poland Polish Acad Sci, Inst Math, PL-00656 Warsaw, Poland Monash Univ, Sch Phys & Astron, Clayton, Vic 3800, Australia Hanyang Univ, Seoul 133791, South Korea Chinese Univ Hong Kong, Shatin, Hong Kong, Peoples R China Univ Alabama Huntsville, Huntsville, AL 35899 USA CNRS, ESPCI, F-75005 Paris, France Univ Minnesota, Minneapolis, MN 55455 USA Univ Camerino, Dipartimento Fis, I-62032 Camerino, Italy Southern Univ & A&M Coll, Baton Rouge, LA 70813 USA Univ Melbourne, Parkville, Vic, Australia Coll William & Mary, Williamsburg, VA 23187 USA Univ Estadual Paulista, Inst Fis Teor, ICTP South Amer Inst Fundament Res, BR-01140070 Sao Paulo, SP, Brazil Whitman Coll, 345 Boyer Ave, Walla Walla, WA 99362 USA Univ Lyon, F-69361 Lyon, France Hobart & William Smith Colleges, Geneva, NY 14456 USA Univ Zielona Gora, Janusz Gil Inst Astron, PL-65265 Zielona Gora, Poland Univ London, Kings Coll London, London WC2R 2LS, England IISER Kolkata, Mohanpur 741252, W Bengal, India Indian Inst Technol, Ahmadabad 382424, Gujarat, India Andrews Univ, Berrien Springs, MI 49104 USA Univ Siena, I-53100 Siena, Italy Trinity Univ, San Antonio, TX 78212 USA Univ Washington, Seattle, WA 98195 USA Abilene Christian Univ, Abilene, TX 79699 USA INFN, Sez Napoli, I-80100 Naples, Italy Univ Estadual Paulista, Inst Fis Teor, ICTP South Amer Inst Fundament Res, BR-01140070 Sao Paulo, SP, Brazil
Published: 2018

6. Incommensurate charge ordered states in the t–t'–J model

Author: Peayush Choubey, Ting-Kuo Lee, Peter Hirschfeld, Wei-Lin Tu, Department of Physics [Gainesville] (UF|Physics), University of Florida [Gainesville] (UF), National Taiwan University, Academia Sinica, Fermions Fortement Corrélés (LPT) (FFC), Laboratoire de Physique Théorique (LPT), Institut de Recherche sur les Systèmes Atomiques et Moléculaires Complexes (IRSAMC), Institut National des Sciences Appliquées - Toulouse (INSA Toulouse), Institut National des Sciences Appliquées (INSA)-Institut National des Sciences Appliquées (INSA)-Centre National de la Recherche Scientifique (CNRS)-Université Toulouse III - Paul Sabatier (UT3), Université Fédérale Toulouse Midi-Pyrénées-Université Fédérale Toulouse Midi-Pyrénées-Institut National des Sciences Appliquées - Toulouse (INSA Toulouse), Université Fédérale Toulouse Midi-Pyrénées-Université Fédérale Toulouse Midi-Pyrénées-Institut de Recherche sur les Systèmes Atomiques et Moléculaires Complexes (IRSAMC), Université Fédérale Toulouse Midi-Pyrénées-Université Fédérale Toulouse Midi-Pyrénées, Université Toulouse III - Paul Sabatier (UT3), Université Fédérale Toulouse Midi-Pyrénées-Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS)-Université Toulouse III - Paul Sabatier (UT3), Université Fédérale Toulouse Midi-Pyrénées-Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche sur les Systèmes Atomiques et Moléculaires Complexes (IRSAMC), Université Fédérale Toulouse Midi-Pyrénées-Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS), Institut National des Sciences Appliquées (INSA)-Institut National des Sciences Appliquées (INSA)-Université Toulouse III - Paul Sabatier (UT3), and Université Fédérale Toulouse Midi-Pyrénées-Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS)-Institut National des Sciences Appliquées - Toulouse (INSA Toulouse)
Subjects: Superconductivity, Physics, Wannier function, Local density of states, Condensed matter physics, General Physics and Astronomy, 02 engineering and technology, 021001 nanoscience & nanotechnology, 01 natural sciences, law.invention, [PHYS.COND.CM-S]Physics [physics]/Condensed Matter [cond-mat]/Superconductivity [cond-mat.supr-con], Amplitude, Mean field theory, law, Condensed Matter::Superconductivity, Pairing, 0103 physical sciences, Scanning tunneling microscope, 010306 general physics, 0210 nano-technology, Charge density wave, ComputingMilieux_MISCELLANEOUS
Abstract: We study the incommensurate charge ordered states in the $\mathit{t-t^{\prime}-J}$ model using the Gutzwiller mean field theory on large systems. In particular, we explore the properties of incommensurate charge modulated states referred to as nodal pair density waves (nPDW) in the literature. nPDW states intertwine site and bond charge order with modulated $d$-wave pair order, and are characterized by a nonzero amplitude of uniform pairing; they also manifest a dominant intra-unit cell $d$-density wave form factor. To compare with a recent scanning tunneling microscopy (STM) study [Hamidian \textit{et al.}, Nat. Phys. 3519 (2015)] of the cuprate superconductor BSCCO-2212, we compute the continuum local density of states (LDOS) at a typical STM tip height using the Wannier function based approach. By Fourier transforming Cu and O sub-lattice LDOS we also obtain bias-dependent intra-unit cell form factors and spatial phase difference. We find that in the nPDW state the behavior of form factors and spatial phase difference as a function of energy agrees remarkably well with the experiment. This is in contrast to commensurate charge modulated states, which we show do not agree with experiment. We propose that the nPDW states are good candidates for the charge density wave phase observed in the superconducting state of underdoped cuprates.
Published: 2017

7. Differentiation of Surface and Bulk Conductivities via Four-probe Spectroscopy

Author: Corentin Durand, Michael A. McGuire, Yang Xu, Yong P. Chen, Xiaoou Zhang, Chuanxu Ma, Ireneusz Miotkowski, An-Ping Li, Saban M. Hus, Helin Cao, Center for Nanophase Materials Sciences [Oak Ridge] (CNMS), Oak Ridge National Laboratory [Oak Ridge] (ORNL), UT-Battelle, LLC-UT-Battelle, LLC, Department of Physics [Gainesville] (UF|Physics), and University of Florida [Gainesville] (UF)
Subjects: Surface (mathematics), Materials science, Analytical chemistry, [PHYS.COND.CM-MS]Physics [physics]/Condensed Matter [cond-mat]/Materials Science [cond-mat.mtrl-sci], 02 engineering and technology, 010402 general chemistry, 021001 nanoscience & nanotechnology, 0210 nano-technology, Spectroscopy, 01 natural sciences, Instrumentation, ComputingMilieux_MISCELLANEOUS, 0104 chemical sciences
Abstract: International audience
Published: 2016

8. Spin-glass-like freezing of inner and outer surface layers in hollow γ-Fe2O3 nanoparticles

Author: Cheng-Jun Sun, Javier Alonso, Manh-Huong Phan, Òscar Iglesias, Paula Lampen-Kelley, Hariharan Srikanth, Hafsa Khurshid, Marie-Louise Saboungi, Department of Physics [Gainesville] (UF|Physics), University of Florida [Gainesville] (UF), Departament de Física Fonamental and Institut de Nanociència i Nanotecnologia, Universitat de Barcelona (UB), BCMaterials Edificio [Derio, Espagne], BCMaterials Edificio, Advanced Photon Source, Argonne National Laboratory, Argonne National Laboratory [Lemont] (ANL), Institut de minéralogie, de physique des matériaux et de cosmochimie (IMPMC), Muséum national d'Histoire naturelle (MNHN)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut de recherche pour le développement [IRD] : UR206-Centre National de la Recherche Scientifique (CNRS), Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut de recherche pour le développement [IRD] : UR206-Muséum national d'Histoire naturelle (MNHN)-Centre National de la Recherche Scientifique (CNRS), and Universitat de Barcelona
Subjects: [PHYS]Physics [physics], Multidisciplinary, Spin glass, Materials science, Nanopartícules, Condensed matter physics, Spins, Magnetic susceptibility, Article, Monte Carlo method, Hysteresis, Magnetization, Exchange bias, Remanence, Vidres de spin, Spin glasses, Nanoparticles, Surface layer, Mètode de Montecarlo
Abstract: Disorder among surface spins is a dominant factor in the magnetic response of magnetic nanoparticle systems. In this work, we examine time-dependent magnetization in high-quality, monodisperse hollow maghemite nanoparticles (NPs) with a 14.8 ± 0.5 nm outer diameter and enhanced surface-to-volume ratio. The nanoparticle ensemble exhibits spin-glass-like signatures in dc magnetic aging and memory protocols and ac magnetic susceptibility. The dynamics of the system slow near 50 K and become frozen on experimental time scales below 20 K. Remanence curves indicate the development of magnetic irreversibility concurrent with the freezing of the spin dynamics. A strong exchange-bias effect and its training behavior point to highly frustrated surface spins that rearrange much more slowly than interior spins. Monte Carlo simulations of a hollow particle corroborate strongly disordered surface layers with complex energy landscapes that underlie both glass-like dynamics and magnetic irreversibility. Calculated hysteresis loops reveal that magnetic behavior is not identical at the inner and outer surfaces, with spins at the outer surface layer of the 15 nm hollow particles exhibiting a higher degree of frustration. Our combined experimental and simulated results shed light on the origin of spin-glass-like phenomena and the important role played by the surface spins in magnetic hollow nanostructures.
Published: 2015

9. Delay-Time and Thermopower Distributions at the Spectrum Edges of a Chaotic Scatterer

Author: Adel Abbout, Jean-Louis Pichard, Geneviève Fleury, Khandker Muttalib, Service de physique de l'état condensé (SPEC - UMR3680), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS), Laboratoire de cristallographie et sciences des matériaux (CRISMAT), École Nationale Supérieure d'Ingénieurs de Caen (ENSICAEN), Normandie Université (NU)-Normandie Université (NU)-Centre National de la Recherche Scientifique (CNRS)-Université de Caen Normandie (UNICAEN), Normandie Université (NU)-Institut de Chimie du CNRS (INC), Department of Physics [Gainesville] (UF|Physics), University of Florida [Gainesville] (UF), Université de Caen Normandie (UNICAEN), Normandie Université (NU)-Normandie Université (NU)-École Nationale Supérieure d'Ingénieurs de Caen (ENSICAEN), Normandie Université (NU)-Institut de Chimie du CNRS (INC)-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche sur les Matériaux Avancés (IRMA), Normandie Université (NU)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université de Rouen Normandie (UNIROUEN), Normandie Université (NU)-Institut national des sciences appliquées Rouen Normandie (INSA Rouen Normandie), Institut National des Sciences Appliquées (INSA)-Normandie Université (NU)-Institut National des Sciences Appliquées (INSA)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université de Rouen Normandie (UNIROUEN), and Institut National des Sciences Appliquées (INSA)-Normandie Université (NU)-Institut National des Sciences Appliquées (INSA)-Centre National de la Recherche Scientifique (CNRS)
Subjects: Gaussian, FOS: Physical sciences, 01 natural sciences, 010305 fluids & plasmas, symbols.namesake, Quantum mechanics, Chaotic scattering, Lattice (order), Mesoscale and Nanoscale Physics (cond-mat.mes-hall), 0103 physical sciences, edge statistics, 010306 general physics, Tracy-Widom, 73.23.-b, 42.25.Bs, 72.20.Pa, 05.45.Mt, [PHYS.COND.CM-MSQHE]Physics [physics]/Condensed Matter [cond-mat]/Mesoscopic Systems and Quantum Hall Effect [cond-mat.mes-hall], Physics, Condensed Matter - Mesoscale and Nanoscale Physics, Condensed matter physics, Scattering, Fermi energy, time-delay matrix, Disordered Systems and Neural Networks (cond-mat.dis-nn), Condensed Matter - Disordered Systems and Neural Networks, Nonlinear Sciences - Chaotic Dynamics, Condensed Matter Physics, Quantum chaos, Electronic, Optical and Magnetic Materials, Cauchy ensemble, Energy distance, chaotic scattering, [NLIN.NLIN-CD]Nonlinear Sciences [physics]/Chaotic Dynamics [nlin.CD], symbols, Embedding, Chaotic Dynamics (nlin.CD), thermopower
Abstract: We study chaotic scattering outside the wide band limit, as the Fermi energy $E_F$ approaches the band edges $E_B$ of a one-dimensional lattice embedding a scattering region of M sites. We show that the delay-time and thermopower distributions differ near the edges from the universal expressions valid in the bulk. To obtain the asymptotic universal forms of these edge distributions, one must keep constant the energy distance $E_F-E_B$ measured in units of the same energy scale proportional to $\propto M^{-1/3}$ which is used for rescaling the energy level spacings at the spectrum edges of large Gaussian matrices. In particular the delay-time and the thermopower have the same universal edge distributions for arbitrary M as those for an M=2 scatterer, which we obtain analytically., Comment: 9 pages, 4 figures
Published: 2013

10. Conductivity map from scanning tunneling potentiometry

Author: Yunmei Chen, Xiaoguang Zhang, Hao Zhang, Corentin Durand, Xianqi Li, An-Ping Li, Department of Mathematics [Gainesville] (UF|Math), University of Florida [Gainesville] (UF), Center for Nanophase Materials Sciences [Oak Ridge] (CNMS), Oak Ridge National Laboratory [Oak Ridge] (ORNL), UT-Battelle, LLC-UT-Battelle, LLC, and Department of Physics [Gainesville] (UF|Physics)
Subjects: Materials science, [PHYS.PHYS]Physics [physics]/Physics [physics], Image registration, 02 engineering and technology, Conductivity, 021001 nanoscience & nanotechnology, 01 natural sciences, Noise (electronics), Computational physics, Conductor, Electrical resistivity and conductivity, 0103 physical sciences, [PHYS.COND.CM-MS]Physics [physics]/Condensed Matter [cond-mat]/Materials Science [cond-mat.mtrl-sci], Grain boundary, 010306 general physics, 0210 nano-technology, Instrumentation, Image restoration, Electrochemical potential
Abstract: International audience; We present a novel method for extracting two-dimensional (2D) conductivity profiles from large electrochemical potential datasets acquired by scanning tunneling potentiometry of a 2D conductor. The method consists of a data preprocessing procedure to reduce/eliminate noise and a numerical conductivity reconstruction. The preprocessing procedure employs an inverse consistent image registration method to align the forward and backward scans of the same line for each image line followed by a total variation (TV) based image restoration method to obtain a (nearly) noise-free potential from the aligned scans. The preprocessed potential is then used for numerical conductivity reconstruction, based on a TV model solved by accelerated alternating direction method of multiplier. The method is demonstrated on a measurement of the grain boundary of a monolayer graphene, yielding a nearly 10:1 ratio for the grain boundary resistivity over bulk resistivity.
Published: 2016

11. The LISA Pathfinder interferometryhardware and system testing

Author: H. Ward, S. Strandmoe, A. Monsky, Gudrun Wanner, M. Schulte, Juan Ramos-Castro, Felipe Guzman, Peter Wass, Gerhard Heinzel, A.M. Taylor, D. Fertin, Walter Fichter, Davor Mance, Michael Perreur-Lloyd, D. Gerardi, C. Trenkel, D. Hoyland, V. Wand, X. Llamas, Matteo Benedetti, Heather Audley, D. Texier, D. Nicolini, A. Perreca, J. A. Romera Perez, B. Rais, C. Boatella, Michele Armano, Eric Plagnol, J. Bogenstahl, Ignacio Mateos, Philippe Jetzer, M. Freschi, Ulrich Johann, Daniele Bortoluzzi, M. Diaz-Aguilo, Karsten Danzmann, F. Pedersen, D. Tombolato, Ivan Lloro, B. Guillaume, D. Shaul, J. Huesler, P. Prat, W. J. Weber, A. Lobo, M. Caleno, J. H. Hough, A. Conchillo, T. J. Sumner, O. Jeannin, I. Harrison, Miquel Nofrarías, Giuseppe D. Racca, D. I. Robertson, Domenico Giardini, F. Antonucci, Frank Steier, Rita Dolesi, M. Cesa, C. García Marirrodriga, M. Cruise, L. Stagnaro, S. Waschke, M. Chmeissani, Mauro Hueller, Stefano Vitale, J. Reiche, I. Cristofolini, Ewan Fitzsimons, G. Dixon, H. Rozemeijer, Pierre Binétruy, B. Johlander, Daniele Nicolodi, S. Madden, A. F. Garcia Marin, Giacomo Ciani, Christian J. Killow, Ingo Diepholz, Peter Zweifel, Antonella Cavalleri, F. De Marchi, P. Luetzow-Wentzky, Catia Grimani, J. Fauste, Lluis Gesa, Oliver Jennrich, G. Auger, Martin Hewitson, Daniel Hollington, R. Maarschalkerweerd, A. Grynagier, Paul McNamara, Gerald Hechenblaikner, J. Sanjuan, Paolo Bosetti, R. Gerndt, F. Gibert, E. Mitchell, José F. F. Mendes, G. Congedo, Luigi Ferraioli, Max-Planck-Institut für Gravitationsphysik ( Albert-Einstein-Institut ) (AEI), Max-Planck-Gesellschaft, EADS Astrium GmbH, Gruppo Collegato di Trento, Istituto Nazionale di Fisica Nucleare (INFN), European Space Astronomy Centre (ESAC), European Space Agency (ESA), AstroParticule et Cosmologie (APC (UMR_7164)), Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), DCT / AQ / EC, Centre National d'Études Spatiales [Toulouse] (CNES), European Space Technology Centre, Institut de Física d’Altes Energies [Barcelone] (IFAE), Universitat Autònoma de Barcelona (UAB), Department of Physics [Gainesville] (UF|Physics), University of Florida [Gainesville] (UF), Facultat de Ciències, Institut d'Estudis Espacials de Catalunya (IEEC-CSIC), School of Physics and Astronomy [Birmingham], University of Birmingham [Birmingham], EPSC, Institut für Flugmechanik und Flugregelung, SUPA School of Physics and Astronomy [Glasgow], University of Glasgow, Institut für Geophysik [Zürich], Eidgenössische Technische Hochschule - Swiss Federal Institute of Technology [Zürich] (ETH Zürich), Istituto di Fisica, INFN Urbino, NASA Goddard Space Flight Center (GSFC), European Space Operations Centre, Blackett Laboratory, Imperial College London, Institut für Theoretische Physik, Universität Zürich [Zürich] = University of Zurich (UZH), NTE-SENER, Departament d'Enginyeria Electrònica [Barcelona], Astrium Ltd, APC - Cosmologie, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, APC - THEORIE, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Institut für theoretische Physik, Universität Hamburg (UHH)-Universität Hamburg (UHH), LISA, Agence Spatiale Européenne = European Space Agency (ESA), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), European Space Research and Technology Centre (ESTEC), National Institute for Nuclear Physics (INFN), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7), Universitat Autònoma de Barcelona [Barcelona] (UAB), Department of Physics [Gainesville], University of Florida [Gainesville], Eidgenössische Technische Hochschule - Swiss Federal Institute of Technology in Zürich [Zürich] (ETH Zürich), Universität Zürich [Zürich] (UZH), Physique Corpusculaire et Cosmologie - Collège de France (PCC), Collège de France (CdF)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Collège de France (CdF)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-AstroParticule et Cosmologie (APC (UMR_7164)), PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, and PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Institut für theoretische Physik
Subjects: Physics, Physics and Astronomy (miscellaneous), 010308 nuclear & particles physics, Integration testing, business.industry, [SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], 99.55.Ym, System testing, 01 natural sciences, 04.80.Nn, 07.60.Ly, Toolbox, Test (assessment), [PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], Interferometry, Pathfinder, 0103 physical sciences, Data analysis, [PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc], 010306 general physics, MATLAB, business, computer, Computer hardware, computer.programming_language
Abstract: International audience; The LISA Pathfinder interferometry- hardware and system testing 2 Abstract. Preparations for the LISA Pathfinder mission have reached an exciting stage. Tests of the engineering model (EM) of the optical metrology system (OMS) have recently been completed at the Albert Einstein Institute, Hannover, and flight model (FM) tests are now underway. Significantly, they represent the first complete integration and testing of the space-qualified hardware and are the first tests on an optical system level. The results and test procedures of these campaigns will be utilised directly in the ground-based flight hardware tests, and subsequently during in-flight operations. In addition, they allow valuable testing of the data analysis methods using the MATLAB based LTP data analysis (LTPDA) toolbox. This paper presents an overview of the results from the EM test campaign that was successfully completed in December 2009. The LISA Pathfinder interferometry- hardware and system testing 3
Published: 2011

12. LISA Pathfinder data analysis

Author: Lluis Gesa, G. Auger, R. Maarschalkerweerd, S. Strandmoe, Ivan Lloro, Gudrun Wanner, Juan Ramos-Castro, X. Llamas, Antonella Cavalleri, Karsten Danzmann, Michele Armano, S. Madden, A. Perreca, D. Fertin, M. Freschi, H. Rozemeijer, I. Harrison, M. Schulte, Ignacio Mateos, M. Cesa, Pierre Binétruy, D. Shaul, D. Texier, Michael Perreur-Lloyd, O. Jeannin, Paolo Bosetti, C. García Marirrodriga, T. J. Sumner, J. Fauste, Felipe Guzman, A. Monsky, B. Guillaume, M. Caleno, Gerhard Heinzel, Ingo Diepholz, D. I. Robertson, M. Chmeissani, Mauro Hueller, P. Prat, Peter Wass, D. Mance, A. Conchillo, Ewan Fitzsimons, A.M. Taylor, J. H. Hough, A. Grynagier, H. Ward, Paul McNamara, A. Lobo, D. Nicolini, D. Tombolato, Giuseppe D. Racca, Matteo Benedetti, F. Antonucci, J. Reiche, C. Trenkel, G. Dixon, G. Congedo, Luigi Ferraioli, J. Huesler, J. A. Romera Perez, Giacomo Ciani, J. Sanjuan, B. Rais, C. Boatella, Eric Plagnol, Domenico Giardini, Frank Steier, M. Diaz-Aguilo, Peter Zweifel, Oliver Jennrich, F. De Marchi, Daniele Bortoluzzi, F. Pedersen, E. Mitchell, José F. F. Mendes, Catia Grimani, Daniele Nicolodi, I. Cristofolini, Philippe Jetzer, Christian J. Killow, Miquel Nofrarías, Rita Dolesi, W. J. Weber, A. F. Garcia Marin, L. Stagnaro, Martin Hewitson, Daniel Hollington, B. Johlander, Heather Audley, S. Waschke, J. Bogenstahl, M. Cruise, Stefano Vitale, Walter Fichter, D. Hoyland, APC - Cosmologie, AstroParticule et Cosmologie (APC (UMR_7164)), Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), APC - THEORIE, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Institut für theoretische Physik, Universität Hamburg (UHH)-Universität Hamburg (UHH), Centre National d'Études Spatiales [Toulouse] (CNES), LISA, Gruppo Collegato di Trento, Istituto Nazionale di Fisica Nucleare (INFN), European Space Astronomy Centre (ESAC), European Space Agency (ESA), Max-Planck-Institut für Gravitationsphysik ( Albert-Einstein-Institut ) (AEI), Max-Planck-Gesellschaft, DCT / AQ / EC, European Space Technology Centre, Institut de Física d’Altes Energies [Barcelone] (IFAE), Universitat Autònoma de Barcelona (UAB), Department of Physics [Gainesville] (UF|Physics), University of Florida [Gainesville] (UF), ICE, Institut d'Estudis Espacials de Catalunya (IEEC-CSIC), School of Physics and Astronomy [Birmingham], University of Birmingham [Birmingham], EPSC, Institut für Flugmechanik und Flugregelung, SUPA School of Physics and Astronomy [Glasgow], University of Glasgow, Institut für Geophysik [Zürich], Eidgenössische Technische Hochschule - Swiss Federal Institute of Technology [Zürich] (ETH Zürich), Istituto di Fisica, INFN Urbino, NASA Goddard Space Flight Center (GSFC), European Space Operations Centre, Blackett Laboratory, Imperial College London, Institut für Theoretische Physik, Universität Zürich [Zürich] = University of Zurich (UZH), NTE-SENER, Université Paris Diderot - Paris 7 (UPD7), Departament d'Enginyeria Electrònica [Barcelona], Astrium Ltd, Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Physique Corpusculaire et Cosmologie - Collège de France (PCC), Collège de France (CdF)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Collège de France (CdF)-Centre National de la Recherche Scientifique (CNRS), PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Institut für theoretische Physik, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7), National Institute for Nuclear Physics (INFN), Universitat Autònoma de Barcelona [Barcelona] (UAB), Department of Physics [Gainesville], University of Florida [Gainesville], Eidgenössische Technische Hochschule - Swiss Federal Institute of Technology in Zürich [Zürich] (ETH Zürich), Universität Zürich [Zürich] (UZH), Agence Spatiale Européenne = European Space Agency (ESA), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), and European Space Research and Technology Centre (ESTEC)
Subjects: Physics, Mission operations, Physics and Astronomy (miscellaneous), 010308 nuclear & particles physics, [SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], 01 natural sciences, Phase (combat), [PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], Noise, Identification (information), Pathfinder, Full data, Physical Sciences, 0103 physical sciences, [PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc], Systems engineering, Key (cryptography), Satellite, 010303 astronomy & astrophysics
Abstract: International audience; As the launch of LISA Pathfinder draws near, more and more effort is being put in to the preparation of the data analysis activities that will be carried out during the mission operations. The operations phase of the mission will be composed of a series of experiments that will be carried out on the satellite. These experiments will be directed and analysed by the data analysis team, which is part of the operations team. The operations phase will last about 90 days, during which time the data analysis team aims to fully characterise the LISA Pathfinder satellite, and in particular, its core instrument the LISA Technology Package. By analysing the various couplings present in the system, the different noise sources that will disturb the system, and through the identification of the key physical parameters of the system, a detailed noise budget of the instrument will be constructed that will allow the performance of the different subsystems to be assessed and projected towards LISA. This paper describes the various aspects of the full data analysis chain that are needed to successfully characterise LPF and build up the noise budget during mission operations.
Published: 2011

13. From laboratory experiments to LISA Pathfinder: achieving LISA geodesic motion

Author: F Antonucci, M Armano, H Audley, G Auger, M Benedetti, P Binetruy, C Boatella, J Bogenstahl, D Bortoluzzi, P Bosetti, N Brandt, M Caleno, A Cavalleri, M Cesa, M Chmeissani, G Ciani, A Conchillo, G Congedo, I Cristofolini, M Cruise, K Danzmann, F De Marchi, M Diaz-Aguilo, I Diepholz, G Dixon, R Dolesi, N Dunbar, J Fauste, L Ferraioli, D Fertin, W Fichter, E Fitzsimons, M Freschi, A García Marin, C García Marirrodriga, R Gerndt, L Gesa, D Giardini, F Gibert, C Grimani, A Grynagier, B Guillaume, F Guzmán, I Harrison, G Heinzel, M Hewitson, D Hollington, J Hough, D Hoyland, M Hueller, J Huesler, O Jeannin, O Jennrich, P Jetzer, B Johlander, C Killow, X Llamas, I Lloro, A Lobo, R Maarschalkerweerd, S Madden, D Mance, I Mateos, P W McNamara, J Mendes, E Mitchell, A Monsky, D Nicolini, D Nicolodi, M Nofrarias, F Pedersen, M Perreur-Lloyd, A Perreca, E Plagnol, P Prat, G D Racca, B Rais, J Ramos-Castro, J Reiche, J A Romera Perez, D Robertson, H Rozemeijer, J Sanjuan, A Schleicher, M Schulte, D Shaul, L Stagnaro, S Strandmoe, F Steier, T J Sumner, A Taylor, D Texier, C Trenkel, D Tombolato, S Vitale, G Wanner, H Ward, S Waschke, P Wass, W J Weber, P Zweifel, Science and Technology Facilities Council (STFC), Gruppo Collegato di Trento, Istituto Nazionale di Fisica Nucleare (INFN), European Space Astronomy Centre (ESAC), European Space Agency (ESA), Max-Planck-Institut für Gravitationsphysik ( Albert-Einstein-Institut ) (AEI), Max-Planck-Gesellschaft, AstroParticule et Cosmologie (APC (UMR_7164)), Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), DCT / AQ / EC, Centre National d'Études Spatiales [Toulouse] (CNES), Astrium GmbH, European Space Technology Centre, Institut de Física d’Altes Energies [Barcelone] (IFAE), Universitat Autònoma de Barcelona (UAB), Department of Physics [Gainesville] (UF|Physics), University of Florida [Gainesville] (UF), Facultat de Ciències, Institut d'Estudis Espacials de Catalunya (IEEC-CSIC), School of Physics and Astronomy [Birmingham], University of Birmingham [Birmingham], EPSC, Astrium Ltd, Institut für Flugmechanik und Flugregelung, SUPA School of Physics and Astronomy [Glasgow], University of Glasgow, Institut für Geophysik [Zürich], Eidgenössische Technische Hochschule - Swiss Federal Institute of Technology [Zürich] (ETH Zürich), Istituto di Fisica, NASA, European Space Operations Centre, Blackett Laboratory, Imperial College London, Dipartimento di Fisica, INFN, Gruppo Collegato di Trento, Institut für Theoretische Physik, Universität Zürich [Zürich] = University of Zurich (UZH), NTE-SENER, Departament d'Enginyeria Electrònica [Barcelona], APC - Cosmologie, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, APC - THEORIE, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Institut für theoretische Physik, Universität Hamburg (UHH)-Universität Hamburg (UHH), LISA, Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Physique Corpusculaire et Cosmologie - Collège de France (PCC), Collège de France (CdF)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Collège de France (CdF)-Centre National de la Recherche Scientifique (CNRS), PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Institut für theoretische Physik, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7), National Institute for Nuclear Physics (INFN), Universitat Autònoma de Barcelona [Barcelona] (UAB), Department of Physics [Gainesville], University of Florida [Gainesville], Eidgenössische Technische Hochschule - Swiss Federal Institute of Technology in Zürich [Zürich] (ETH Zürich), Universität Zürich [Zürich] (UZH), Agence Spatiale Européenne = European Space Agency (ESA), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), and European Space Research and Technology Centre (ESTEC)
Subjects: Ground testing, [PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM], Geodesic, Physics and Astronomy (miscellaneous), [SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], FOS: Physical sciences, General Relativity and Quantum Cosmology (gr-qc), 01 natural sciences, Motion (physics), General Relativity and Quantum Cosmology, [PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], Acceleration, 0103 physical sciences, Quantitative assessment, Aerospace engineering, ASTRONOMY & ASTROPHYSICS, 010306 general physics, Instrumentation and Methods for Astrophysics (astro-ph.IM), 01 Mathematical Sciences, MISSION, Physics, Science & Technology, PHYSICS, MULTIDISCIPLINARY, 02 Physical Sciences, 010308 nuclear & particles physics, business.industry, PHYSICS, PARTICLES & FIELDS, Nuclear & Particles Physics, Noise, Pathfinder, Physical Sciences, [PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc], business, Astrophysics - Instrumentation and Methods for Astrophysics
Abstract: This paper presents a quantitative assessment of the performance of the upcoming LISA Pathfinder geodesic explorer mission. The findings are based on the results of extensive ground testing and simulation campaigns using flight hardware and flight control and operations algorithms. The results show that, for the central experiment of measuring the stray differential acceleration between the LISA test masses, LISA Pathfinder will be able to verify the overall acceleration noise to within a factor two of the LISA requirement at 1 mHz and within a factor 6 at 0.1 mHz. We also discuss the key elements of the physical model of disturbances, coming from LISA Pathfinder and ground measurement, that will guarantee the LISA performance., Proceedings of the 8th LISA Symposium. To appear Class. Quantum Grav. 28 (2011)
Published: 2011

14. LISA Pathfinder: mission and status

Author: Antonucci, F, Armano, M, Audley, H, Auger, G, Benedetti, M, Binetruy, P, Boatella, C, Bogenstahl, J, Bortoluzzi, D, Bosetti, P, Caleno, M, Cavalleri, A, Cesa, M, Chmeissani, M, Ciani, G, Conchillo, A, Congedo, G, Cristofolini, I, Cruise, M, Danzmann, K, De Marchi, F, Diaz-Aguilo, M, Diepholz, I, Dixon, G, Dolesi, R, Dunbar, N, Fauste, J, Ferraioli, L, Fertin, D, Fichter, W, Fitzsimons, E, Freschi, M, Marin, AG, Marirrodriga, CG, Gerndt, R, Gesa, L, Gilbert, F, Giardini, D, Grimani, C, Grynagier, A, Guillaume, B, Guzmán, F, Harrison, I, Heinzel, G, Hewitson, M, Hollington, D, Hough, J, Hoyland, D, Hueller, M, Huesler, J, Jeannin, O, Jennrich, O, Jetzer, P, Johlander, B, Killow, C, Llamas, X, Lloro, I, Lobo, A, Maarschalkerweerd, R, Madden, S, Mance, D, Mateos, I, McNamara, PW, Mendes, J, Mitchell, E, Monsky, A, Nicolini, D, Nicolodi, D, Nofrarias, M, Pedersen, F, Perreur-Lloyd, M, Perreca, A, Plagnol, E, Prat, P, Racca, GD, Rais, B, Ramos-Castro, J, Reiche, J, Perez, JAR, Robertson, D, Rozemeijer, H, Sanjuan, J, Schleicher, A, Schulte, M, Shaul, D, Stagnaro, L, Strandmoe, S, Steier, F, Sumner, TJ, Taylor, A, Texier, D, Trenkel, C, Tombolato, D, Vitale, S, Wanner, G, Ward, H, Waschke, S, Wass, P, Weber, WJ, Zweifel, P, Gruppo Collegato di Trento, National Institute for Nuclear Physics ( INFN ), European Space Astronomy Centre, European Space Agency ( ESA ), Max-Planck-Institut für Gravitationsphysik, Universitat Hannover, AstroParticule et Cosmologie ( APC - UMR 7164 ), Centre National de la Recherche Scientifique ( CNRS ) -Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Observatoire de Paris-Université Paris Diderot - Paris 7 ( UPD7 ) -Commissariat à l'énergie atomique et aux énergies alternatives ( CEA ), Centre National d'Etudes Spatiales ( CNES ), European Space Technology Centre, IFAE, Universitat Autònoma de Barcelona [Barcelona] ( UAB ), Department of Physics [Gainesville], University of Florida [Gainesville], ICE, Institut d'Estudis Espacials de Catalunya ( IEEC-CSIC ), School of Physics and Astronomy [Birmingham], University of Birmingham [Birmingham], EPSC, Astrium Ltd, Institut für Flugmechanik und Flugregelung, Department of Physics and Astronomy, University of Glasgow, Astrium GmbH, Institut für Geophysik [Zürich], Eidgenössische Technische Hochschule [Zürich] ( ETH Zürich ), Istituto di Fisica, NASA Goddard Space Flight Center ( GSFC ), European Space Operations Centre, Blackett Laboratory, Imperial College London, Institut für Theoretische Physik, Universität Zürich [Zürich] ( UZH ), NTE-SENER, Departament d'Enginyeria Electrònica [Barcelona], Istituto Nazionale di Fisica Nucleare (INFN), European Space Astronomy Centre (ESAC), Agence Spatiale Européenne = European Space Agency (ESA), Max-Planck-Institut für Gravitationsphysik ( Albert-Einstein-Institut ) (AEI), Max-Planck-Gesellschaft, AstroParticule et Cosmologie (APC (UMR_7164)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Centre National d'Études Spatiales [Toulouse] (CNES), European Space Research and Technology Centre (ESTEC), Institut de Física d’Altes Energies [Barcelone] (IFAE), Universitat Autònoma de Barcelona (UAB), Department of Physics [Gainesville] (UF|Physics), University of Florida [Gainesville] (UF), Institut d'Estudis Espacials de Catalunya (IEEC-CSIC), SUPA School of Physics and Astronomy [Glasgow], Eidgenössische Technische Hochschule - Swiss Federal Institute of Technology [Zürich] (ETH Zürich), NASA Goddard Space Flight Center (GSFC), Universität Zürich [Zürich] = University of Zurich (UZH), National Institute for Nuclear Physics (INFN), European Space Agency (ESA), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7), Universitat Autònoma de Barcelona [Barcelona] (UAB), Eidgenössische Technische Hochschule - Swiss Federal Institute of Technology in Zürich [Zürich] (ETH Zürich), Universität Zürich [Zürich] (UZH), Observatoire de Paris, and Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)
Subjects: Physics and Astronomy (miscellaneous), Physical Sciences, [PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc], ComputingMilieux_MISCELLANEOUS, [ PHYS.GRQC ] Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]
Abstract: LISA Pathfinder, the second of the European Space Agency's Small Missions for Advanced Research in Technology (SMART), is a dedicated technology demonstrator for the joint ESA/NASA Laser Interferometer Space Antenna (LISA) mission. The technologies required for LISA are many and extremely challenging. This coupled with the fact that some flight hardware cannot be fully tested on ground due to Earth-induced noise led to the implementation of the LISA Pathfinder mission to test the critical LISA technologies in a flight environment. LISA Pathfinder essentially mimics one arm of the LISA constellation by shrinking the 5 million kilometre armlength down to a few tens of centimetres, giving up the sensitivity to gravitational waves, but keeping the measurement technology: the distance between the two test masses is measured using a laser interferometric technique similar to one aspect of the LISA interferometry system. The scientific objective of the LISA Pathfinder mission consists then of the first in-flight test of low frequency gravitational wave detection metrology. LISA Pathfinder is due to be launched in 2013 on-board a dedicated small launch vehicle (VEGA). After a series of apogee raising manoeuvres using an expendable propulsion module, LISA Pathfinder will enter a transfer orbit towards the first Sun-Earth Lagrange point (L1). After separation from the propulsion module, the LPF spacecraft will be stabilized using the micro-Newton thrusters, entering a 500 000 km by 800 000 km Lissajous orbit around L1. Science results will be available approximately 2 months after launch. © 2011 IOP Publishing Ltd.
Published: 2011

15. The Casimir force on a surface with shallow nanoscale corrugations: Geometry and finite conductivity effects

Author: Y. Bao, Ho Bun Chan, Astrid Lambrecht, Chien-Shing Pai, Raymond A. Cirelli, Romain Guérout, F.P. Klemens, J. Lussange, William M. Mansfield, Department of Physics [Gainesville] (UF|Physics), University of Florida [Gainesville] (UF), Laboratoire Kastler Brossel (LKB (Jussieu)), Université Pierre et Marie Curie - Paris 6 (UPMC)-Fédération de recherche du Département de physique de l'Ecole Normale Supérieure - ENS Paris (FRDPENS), École normale supérieure - Paris (ENS Paris), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-École normale supérieure - Paris (ENS Paris), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Centre National de la Recherche Scientifique (CNRS), Bell Laboratories, Alcatel-Lucent, Bell Laboratories, Department of Physics [Hong Kong University of Science and Technology], Hong Kong University of Science and Technology (HKUST), Fédération de recherche du Département de physique de l'Ecole Normale Supérieure - ENS Paris (FRDPENS), École normale supérieure - Paris (ENS-PSL), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-École normale supérieure - Paris (ENS-PSL), and Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Centre National de la Recherche Scientifique (CNRS)
Subjects: Physics, Surface (mathematics), Quantum Physics, Nanostructure, Silicon, 010308 nuclear & particles physics, Scattering, General Physics and Astronomy, chemistry.chemical_element, FOS: Physical sciences, Geometry, 01 natural sciences, Semimetal, Casimir effect, chemistry, [PHYS.QPHY]Physics [physics]/Quantum Physics [quant-ph], 0103 physical sciences, Scattering theory, 010306 general physics, Quantum Physics (quant-ph), Nanoscopic scale
Abstract: International audience; We measure the Casimir force between a gold sphere and a silicon plate with nanoscale, rectangular corrugations with depth comparable to the separation between the surfaces. In the proximity force approximation (PFA), both the top and bottom surfaces of the corrugations contribute to the force, leading to a distance dependence that is distinct from a flat surface. The measured Casimir force is found to deviate from the PFA by up to 15%, in good agreement with calculations based on scattering theory that includes both geometry effects and the optical properties of the material.
Published: 2010

16. Quasiparticle Fock-space Coupled-cluster Theory

Author: Hendrik J. Monkhorst, Leszek Z. Stolarczyk, Faculty of Chemistry [Warsaw], University of Warsaw (UW), Department of Physics [Gainesville] (UF|Physics), and University of Florida [Gainesville] (UF)
Subjects: Physics, 010304 chemical physics, Antisymmetric relation, Biophysics, Unitary transformation, Condensed Matter Physics, 01 natural sciences, Fock space, Theoretical physics, Fock state, Multiplication operator, Operator algebra, Particle number operator, Quantum mechanics, 0103 physical sciences, Physical Sciences, Quasiparticle, Physical and Theoretical Chemistry, 010306 general physics, Molecular Biology
Abstract: International audience; The quasiparticle Fock-space coupled-cluster (QFSCC) theory, introduced by us in 1985, is described. This is a theory of many-electron systems which uses the second-quantization formalism based on the algebraic approximation: one chooses a finite spin-orbital basis, and builds a fermionic Fock space to represent all possible antisymmetric electronic states of a given system. The algebraic machinery is provided by the algebra of linear operators acting in the Fock space, generated by the fermion (creation and annihilation) operators. The Fock-space Hamiltonian operator then determines the system's stationary states and their energies. Within the QFSCC theory, the Fock space and its operator algebra are subject to a unitary transformation which effectively changes electrons into some fermionic quasiparticles. A generalization of the coupled-cluster method is achieved by enforcing the principle of quasiparticle-number conservation. The emerging quasiparticle model of many-electron systems offers useful physical insights and computational effectiveness. The QFSCC theory requires a substantial reformulation of the traditional second-quantization language, by making a full use of the algebraic properties of the Fock space and its operator algebra. In particular, the role of operators not conserving the number of electrons (or quasiparticles) is identified.
Published: 2010

17. Density Diagnostic Using Stark Broadening of He I Spectral Line Emission from Rydberg Levels

Author: Y. Marandet, L. Godbert-Mouret, M. Koubiti, Roland Stamm, Frank B. Rosmej, A. Meigs, Joël Rosato, H. Capes, Physique des interactions ioniques et moléculaires (PIIM), Aix Marseille Université (AMU)-Centre National de la Recherche Scientifique (CNRS), Département de Recherche sur la Fusion Contrôlée (DRFC), Commissariat à l'énergie atomique et aux énergies alternatives (CEA), Department of Physics [Gainesville] (UF|Physics), University of Florida [Gainesville] (UF), UKAEA-Euratom (UKAEA-Euratom), and UKAEA-EURATOM
Subjects: Physics, Balmer series, Condensed Matter Physics, 01 natural sciences, 7. Clean energy, Spectral line, 010305 fluids & plasmas, symbols.namesake, Dipole, Stark effect, Einstein coefficients, [PHYS.PHYS.PHYS-PLASM-PH]Physics [physics]/Physics [physics]/Plasma Physics [physics.plasm-ph], 0103 physical sciences, symbols, Rydberg formula, Plasma diagnostics, Physics::Atomic Physics, Atomic physics, 010306 general physics, ComputingMilieux_MISCELLANEOUS, Line (formation)
Abstract: Neutral helium line spectra of the diffuse series observed under recombining plasma conditions, are used for electron density diagnostics. The method is similar to that using high members of the Balmer series of hydrogen or its isotopes. It is based on the comparison of experimental line spectra to calculated Stark profiles obtained with the Stark line shape code PPP. Among the required atomic data, the dipole reduced matrix elements have been calculated using a hydrogenic approximation. A good agreement was found between the behaviors of the Einstein coefficients calculated using this approximation and the available corresponding values found in the literature. It is demonstrated here through its application to JET data that for relatively dense plasmas this method gives promising results which are consistent with other measurements.
Published: 2006

18. Optimisation de la génération d'harmoniques d'ordre élevé à l'aide d'une optique adaptative et d'un modulateur acousto-optique

Author: O. Boyko, Th. A. Planchon, Constance Valentin, David H. Reitze, Sophie Kazamias, Ph. Balcou, Laboratoire d'optique appliquée (LOA), École Nationale Supérieure de Techniques Avancées (ENSTA Paris)-École polytechnique (X)-Centre National de la Recherche Scientifique (CNRS), Department of Physics [Gainesville] (UF|Physics), University of Florida [Gainesville] (UF), Laboratoire d'interaction du rayonnement X avec la matière (LIXAM), and Université Paris-Sud - Paris 11 (UP11)-Centre National de la Recherche Scientifique (CNRS)
Subjects: [PHYS.PHYS.PHYS-OPTICS]Physics [physics]/Physics [physics]/Optics [physics.optics], 0103 physical sciences, General Physics and Astronomy, 01 natural sciences, 010305 fluids & plasmas
Abstract: International audience; Afin de contrôler la génération d'harmoniques d'ordre élevé dans des conditions optimisées, nous avons réalisé des expériences préliminaires de contrôle spectral et spatial du laser infrarouge. Nous avons démontré la possibilité de modifier la longueur d'onde des harmoniques grâce à la modification de la phase spectrale du laser infrarouge par un modulateur acousto-optique « Dazzler ». Nous montrons que cette méthode permet d'obtenir un spectre plus large et un flux de photon intégré beaucoup plus important qu'en utilisant une simple modification de la dérive de fréquence du laser. Nous présentons également les premiers résultats de mise en forme de la tache focale du laser par optique adaptative, et l'effet de ce contrôle spatial sur la génération d‘harmoniques.
Published: 2005

19. Spectral tailoring of high harmonic generation by adaptative methods

Author: Boyko, O., Planchon, Th A., Constance Valentin, Douillet, D., Reitze, D., Kazamias, S., Stéphane Sebban, Philippe Balcou, Laboratoire d'optique appliquée (LOA), École Nationale Supérieure de Techniques Avancées (ENSTA Paris)-École polytechnique (X)-Centre National de la Recherche Scientifique (CNRS), Department of Physics [Gainesville] (UF|Physics), University of Florida [Gainesville] (UF), Laboratoire d'interaction du rayonnement X avec la matière (LIXAM), and Université Paris-Sud - Paris 11 (UP11)-Centre National de la Recherche Scientifique (CNRS)
Subjects: [PHYS.PHYS.PHYS-OPTICS]Physics [physics]/Physics [physics]/Optics [physics.optics]
Abstract: International audience; In this paper, we present two methods for optimizing the process of high-harmonic generation. The first one consists in affecting the spectral phase of a driving laser using an acoustic–optical programmable dispersive filter called “Dazzler.” By this method we have shown an enhancement of the efficiency and tuning of high-order harmonics. We also present a method for shaping the intensity distribution of an intense laser beam in the focal region by means of a bimorph adaptive mirror. First results on the control of harmonic spectra obtained with shaped intensity profiles are presented.

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19 results on '"Department of Physics [Gainesville] (UF|Physics)"'

1. Prompt gravity signal induced by the 2011 Tohoku-Oki earthquake

2. Earthquake early warning using future generation gravity strainmeters

3. Using controlled disorder to probe the interplay between charge order and superconductivity in NbSe$_2$

4. Differentiation of Surface and Bulk Conductivities in Topological Insulators via Four-Probe Spectroscopy

5. All-sky search for long-duration gravitational wave transients in the first Advanced LIGO observing run

6. Incommensurate charge ordered states in the t–t'–J model

7. Differentiation of Surface and Bulk Conductivities via Four-probe Spectroscopy

8. Spin-glass-like freezing of inner and outer surface layers in hollow γ-Fe2O3 nanoparticles

9. Delay-Time and Thermopower Distributions at the Spectrum Edges of a Chaotic Scatterer

10. Conductivity map from scanning tunneling potentiometry

11. The LISA Pathfinder interferometryhardware and system testing

12. LISA Pathfinder data analysis

13. From laboratory experiments to LISA Pathfinder: achieving LISA geodesic motion

14. LISA Pathfinder: mission and status

15. The Casimir force on a surface with shallow nanoscale corrugations: Geometry and finite conductivity effects

16. Quasiparticle Fock-space Coupled-cluster Theory

17. Density Diagnostic Using Stark Broadening of He I Spectral Line Emission from Rydberg Levels

18. Optimisation de la génération d'harmoniques d'ordre élevé à l'aide d'une optique adaptative et d'un modulateur acousto-optique

19. Spectral tailoring of high harmonic generation by adaptative methods

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19 results on '"Department of Physics [Gainesville] (UF|Physics)"'

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