GW150914: The advanced LIGO detectors in the era of first discoveries

dc.contributorCalifornia Institute of Technology
dc.contributorLouisiana State University
dc.contributorUniversità di Salerno
dc.contributorComplesso Universitario di Monte sant'Angelo
dc.contributorUniversity of Florida
dc.contributorLIGO Livingston Observatory
dc.contributorCNRS/IN2P3
dc.contributorMax-Planck-Institut für Gravitationsphysik
dc.contributorScience Park
dc.contributorMassachusetts Institute of Technology
dc.contributorInstituto Nacional de Pesquisas Espaciais
dc.contributorGran Sasso Science Institute
dc.contributorSezione di Roma Tor Vergata
dc.contributorInter-University Centre for Astronomy and Astrophysics
dc.contributorTata Institute of Fundamental Research
dc.contributorUniversity of Wisconsin-Milwaukee
dc.contributorLeibniz Universität Hannover
dc.contributorUniversità di Pisa
dc.contributorSezione di Pisa
dc.contributorAustralian National University
dc.contributorUniversity of Mississippi
dc.contributorCalifornia State University Fullerton
dc.contributorUniversité Paris-Saclay
dc.contributorChennai Mathematical Institute
dc.contributorUniversità di Roma Tor Vergata
dc.contributorUniversity of Southampton
dc.contributorUniversität Hamburg
dc.contributorSezione di Roma
dc.contributorSorbonne Paris Cité
dc.contributorMontana State University
dc.contributorUniversità di Perugia
dc.contributorSezione di Perugia
dc.contributorEuropean Gravitational Observatory (EGO)
dc.contributorSyracuse University
dc.contributorUniversity of Glasgow
dc.contributorLIGO Hanford Observatory
dc.contributorRMKI
dc.contributorColumbia University
dc.contributorStanford University
dc.contributorDipartimento di Fisica e Astronomia
dc.contributorSezione di Padova
dc.contributorCAMK-PAN
dc.contributorUniversity of Birmingham
dc.contributorUniversità degli Studi di Genova
dc.contributorSezione di Genova
dc.contributorRRCAT
dc.contributorLomonosov Moscow State University
dc.contributorUniversity of the West of Scotland
dc.contributorUniversity of Western Australia
dc.contributorRadboud University Nijmegen
dc.contributorObservatoire Côte d'Azur
dc.contributorLendulet Astrophysics Research Group
dc.contributorUniversité de Rennes 1
dc.contributorWashington State University
dc.contributorUniversità degli Studi di Urbino Carlo Bo
dc.contributorSezione di Firenze
dc.contributorUniversity of Oregon
dc.contributorCollège de France
dc.contributorAstronomical Observatory Warsaw University
dc.contributorVU University Amsterdam
dc.contributorUniversity of Maryland
dc.contributorGeorgia Institute of Technology
dc.contributorUMR CNRS 5306
dc.contributorUniversité de Lyon
dc.contributorIAC3 - IEEC
dc.contributorNASA/Goddard Space Flight Center
dc.contributorUniversity of Toronto
dc.contributorTsinghua University
dc.contributorTexas Tech University
dc.contributorPennsylvania State University
dc.contributorNational Tsing Hua University
dc.contributorCharles Sturt University
dc.contributorUniversity of Chicago
dc.contributorCaltech CaRT
dc.contributorKorea Institute of Science and Technology Information
dc.contributorCarleton College
dc.contributorUniversità di Roma la Sapienza
dc.contributorUniversity of Brussels
dc.contributorSonoma State University
dc.contributorNorthwestern University
dc.contributorUniversity of Minnesota
dc.contributorUniversity of Melbourne
dc.contributorUniversity of Texas Rio Grande Valley
dc.contributorUniversity of Sheffield
dc.contributorUniversity of Sannio at Benevento
dc.contributorMontclair State University
dc.contributorDipartimento di Fisica
dc.contributorTrento Institute for Fundamental Physics and Applications
dc.contributorCardiff University
dc.contributorNational Astronomical Observatory of Japan
dc.contributorUniversity of Edinburgh
dc.contributorGandhinagar Ahmedabad
dc.contributorInstitute for Plasma Research
dc.contributorUniversity of Szeged
dc.contributorEmbry-Riddle Aeronautical University
dc.contributorUniversity of Michigan
dc.contributorAmerican University
dc.contributorUniversity of Massachusetts-Amherst
dc.contributorUniversity of Adelaide
dc.contributorWest Virginia University
dc.contributorUniversity of Biał Ystok
dc.contributorUniversity of Strathclyde
dc.contributorCET Campus
dc.contributorInstitute of Applied Physics
dc.contributorPusan National University
dc.contributorHanyang University
dc.contributorNCBJ
dc.contributorIM-PAN
dc.contributorRochester Institute of Technology
dc.contributorMonash University
dc.contributorSeoul National University
dc.contributorUniversity of Alabama in Huntsville
dc.contributorCNRS
dc.contributorAandM College
dc.contributorCollege of William and Mary
dc.contributorUniversidade Estadual Paulista (UNESP)
dc.contributorUniversity of Cambridge
dc.contributorIISER-Kolkata
dc.contributorHSIC
dc.contributorWhitman College
dc.contributorNational Institute for Mathematical Sciences
dc.contributorHobart and William Smith Colleges
dc.contributorUniversity of Zielona Góra
dc.contributorAndrews University
dc.contributorUniversità di Siena
dc.contributorTrinity University
dc.contributorUniversity of Washington
dc.contributorKenyon College
dc.contributorAbilene Christian University
dc.contributorSezione di Napoli
dc.date.accessioned2022-04-29T07:32:47Z
dc.date.accessioned2022-12-20T02:35:12Z
dc.date.available2022-04-29T07:32:47Z
dc.date.available2022-12-20T02:35:12Z
dc.date.created2022-04-29T07:32:47Z
dc.date.issued2016-03-31
dc.identifierPhysical Review Letters, v. 116, n. 13, 2016.
dc.identifier1079-7114
dc.identifier0031-9007
dc.identifierhttp://hdl.handle.net/11449/228139
dc.identifier10.1103/PhysRevLett.116.131103
dc.identifier2-s2.0-84962845315
dc.identifier.urihttps://repositorioslatinoamericanos.uchile.cl/handle/2250/5408274
dc.description.abstractFollowing a major upgrade, the two advanced detectors of the Laser Interferometer Gravitational-wave Observatory (LIGO) held their first observation run between September 2015 and January 2016. With a strain sensitivity of 10-23/Hz at 100 Hz, the product of observable volume and measurement time exceeded that of all previous runs within the first 16 days of coincident observation. On September 14, 2015, the Advanced LIGO detectors observed a transient gravitational-wave signal determined to be the coalescence of two black holes [B. P. Abbott et al., Phys. Rev. Lett. 116, 061102 (2016)], launching the era of gravitational-wave astronomy. The event, GW150914, was observed with a combined signal-to-noise ratio of 24 in coincidence by the two detectors. Here, we present the main features of the detectors that enabled this observation. At full sensitivity, the Advanced LIGO detectors are designed to deliver another factor of 3 improvement in the signal-to-noise ratio for binary black hole systems similar in mass to GW150914.
dc.languageeng
dc.relationPhysical Review Letters
dc.sourceScopus
dc.titleGW150914: The advanced LIGO detectors in the era of first discoveries
dc.typeArtículos de revistas


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