Quantum correlation measurements in interferometric gravitational-wave detectors
Д. В. Мартынов(Massachusetts Institute of Technology), V. V. Frolov(LIGO Scientific Collaboration), S. Kandhasamy(University of Mississippi), K. Izumi, H. Miao(University of Birmingham), Nergis Mavalvala(Massachusetts Institute of Technology), E. D. Hall(California Institute of Technology), R. K. Lanza(Massachusetts Institute of Technology), B. P. Abbott(California Institute of Technology), R. Abbott(California Institute of Technology), T. D. Abbott(Louisiana State University), C. Adams(LIGO Scientific Collaboration), R. X. Adhikari(California Institute of Technology), S. B. Anderson(California Institute of Technology), A. Ananyeva(California Institute of Technology), S. Appert(California Institute of Technology), K. Arai(California Institute of Technology), S. M. Aston(LIGO Scientific Collaboration), S. Ballmer(Syracuse University), D. Barker, B. Barr(University of Glasgow), L. Barsotti(Massachusetts Institute of Technology), J. Bartlett, I. Bartos(Columbia University), J. C. Batch, A. S. Bell(University of Glasgow), J. Betzwieser(LIGO Scientific Collaboration), G. Billingsley(California Institute of Technology), J. Birch(LIGO Scientific Collaboration), Sébastien Biscans(California Institute of Technology), C. Biwer(Syracuse University), C. D. Blair(The University of Western Australia), R. Bork(California Institute of Technology), A. F. Brooks(California Institute of Technology), G. Ciani(University of Florida), F. Clara, S. T. Countryman(Columbia University), M. J. Cowart(LIGO Scientific Collaboration), D. C. Coyne(California Institute of Technology), A. Cumming(University of Glasgow), L. Cunningham(University of Glasgow), K. Danzmann(Leibniz University Hannover), C. F. Da Silva Costa(University of Florida), E. J. Daw(University of Sheffield), D. DeBra(Stanford University), R. T. DeRosa(LIGO Scientific Collaboration), R. DeSalvo(University of Sannio), K. L. Dooley(University of Mississippi), S. Doravari(LIGO Scientific Collaboration), J. C. Driggers, S. E. Dwyer, A. Effler(LIGO Scientific Collaboration), T. Etzel(California Institute of Technology), M. Evans(Massachusetts Institute of Technology), T. Evans(LIGO Scientific Collaboration), M. Factourovich(Columbia University), H. Fair(Syracuse University), A. Fernández Galiana(Massachusetts Institute of Technology), R. P. Fisher(Syracuse University), P. Fritschel(Massachusetts Institute of Technology), P. Fulda(University of Florida), M. Fyffe(LIGO Scientific Collaboration), J. A. Giaime(Louisiana State University), K. D. Giardina(LIGO Scientific Collaboration), E. Goetz(Max Planck Institute for Gravitational Physics), E. Goetz(University of Florida), S. Gras(Massachusetts Institute of Technology), C. Gray, H. Grote(Max Planck Institute for Gravitational Physics), K. E. Gushwa(California Institute of Technology), E. K. Gustafson(California Institute of Technology), R. Gustafson(University of Michigan), G. Hammond(University of Glasgow), J. Hanks, J. Hanson(LIGO Scientific Collaboration), T. Hardwick(Louisiana State University), I. W. Harry(American University), M. C. Heintze(LIGO Scientific Collaboration), A. W. Heptonstall(California Institute of Technology), J. Hough(University of Glasgow), R. Jones(University of Glasgow), S. Karki(University of Oregon), M. Kasprzack(Louisiana State University), S. Kaufer(Leibniz University Hannover), K. Kawabe, N. Kijbunchoo, E. J. King(The University of Adelaide), Peter King, J. S. Kissel, W. Z. Korth(California Institute of Technology), A. Królak(Max Planck Institute for Gravitational Physics), M. Landry, B. Lantz(Stanford University), N. A. Lockerbie(University of Strathclyde), M. Lormand(LIGO Scientific Collaboration), A. P. Lundgren(Max Planck Institute for Gravitational Physics), M. MacInnis(Massachusetts Institute of Technology), D. M. Macleod(Louisiana State University), Szabolcs Márka(Columbia University), Z. Márka(Columbia University), A. S. Markosyan(Stanford University), E. Maros(California Institute of Technology), I. W. Martin(University of Glasgow), K. Mason(Massachusetts Institute of Technology), T. J. Massinger(Syracuse University), F. Matichard(California Institute of Technology), R. McCarthy, D. E. McClelland(Australian National University), S. McCormick(LIGO Scientific Collaboration), G. McIntyre(California Institute of Technology), J. McIver(California Institute of Technology), G. Mendell, E. L. Merilh, P. M. Meyers(University of Minnesota), J. Miller(Massachusetts Institute of Technology), R. Mittleman(Massachusetts Institute of Technology), G. Moreno, G. Mueller(University of Florida), A. Mullavey(LIGO Scientific Collaboration), J. Münch(The University of Adelaide), L. K. Nuttall(Syracuse University), J. Oberling, P. Oppermann(Max Planck Institute for Gravitational Physics), Richard J. Oram(LIGO Scientific Collaboration), B. O’Reilly(LIGO Scientific Collaboration), D. J. Ottaway(The University of Adelaide), H. Overmier(LIGO Scientific Collaboration), J. R. Palamos(University of Oregon), H. R. Paris(Stanford University), W. Parker(LIGO Scientific Collaboration), A. Pele(LIGO Scientific Collaboration), S. Penn(Hobart and William Smith Colleges), M. Phelps(University of Glasgow), V. Pierro(University of Sannio), I. M. Pinto(University of Sannio), M. Principe(University of Sannio), L. Prokhorov(Lomonosov Moscow State University), O. Puncken(Max Planck Institute for Gravitational Physics), V. Quetschke(The University of Texas Rio Grande Valley), E. A. Quintero(California Institute of Technology), F. J. Raab, H. Radkins, P. Raffai(Eötvös Loránd University), S. Reid(University of the West of Scotland), D. H. Reitze(California Institute of Technology), N. A. Robertson(California Institute of Technology), J. G. Rollins(California Institute of Technology), V. J. Roma(University of Oregon), J. H. Romie(LIGO Scientific Collaboration), S. Rowan(University of Glasgow), K. Ryan, E. Ruiz Morales, E. J. Sanchez(California Institute of Technology), V. Sandberg, R. L. Savage, R. M. S. Schofield(University of Oregon), James A. Sellers(LIGO Scientific Collaboration), D. A. Shaddock(Australian National University), Thomas Shaffer, B. Shapiro(Stanford University), P. Shawhan(University of Maryland, College Park), D. H. Shoemaker(Massachusetts Institute of Technology), D. Sigg, B. J. J. Slagmolen(Australian National University), J. R. Smith(LIGO Scientific Collaboration), J. R. Smith(California State University, Fullerton), B. Sorazu(University of Glasgow), A. Staley(Columbia University), K. A. Strain(University of Glasgow), D. B. Tanner(University of Florida), R. Taylor(California Institute of Technology), M. Thomas(LIGO Scientific Collaboration), P. Thomas, K. A. Thorne(LIGO Scientific Collaboration), E. Thrane(Monash University), C. I. Torrie(California Institute of Technology), G. Traylor(LIGO Scientific Collaboration), G. Vajente(California Institute of Technology), G. Valdes(The University of Texas Rio Grande Valley), A. A. van Veggel(University of Glasgow), A. Vecchio(University of Birmingham), J. Veitch(The University of Adelaide), K. Venkateswara(University of Washington), T. Vo(Syracuse University), C. Vorvick, M. Walker(Louisiana State University), R. L. Ward(Australian National University), J. Warner, B. Weaver, R. Weiss(Massachusetts Institute of Technology), P. Weßels(Max Planck Institute for Gravitational Physics), B. Willke(Leibniz University Hannover), C. C. Wipf(California Institute of Technology), J. Worden, Guanglei Wu(LIGO Scientific Collaboration), H. Yamamoto(California Institute of Technology), C. C. Yancey(University of Maryland, College Park), Hang Yu(Massachusetts Institute of Technology), Haocun Yu(Massachusetts Institute of Technology), L. Zhang(California Institute of Technology), M. E. Zucker(California Institute of Technology), J. Zweizig(California Institute of Technology), LSC Instrument Authors
Cited by 24Open Access
Abstract
A detailed experimental investigation of classical and quantum noises in the LIGO gravitational-wave detector is performed. As a result, an estimate of the quantum radiation pressure noise is given and the sensitivity for the next run of astrophysical experiments is established.
Related Papers
No related papers found
Powered by citation graph analysis