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Tests of General Relativity with GW150914

2016· article· en· 1,800 citations· W2273892807 on OpenAlex· 10.1103/physrevlett.116.221101

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Opus teacher head0.016
GPT teacher head0.349
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0.333 · how far apart the two teachers sit on this one work
Validation status
score_only:v0-immature-baseline · verbatim from the scoring run: score_only means the number may rank works, and no category label ships from it

Abstract

The LIGO detection of GW150914 provides an unprecedented opportunity to study the two-body motion of a compact-object binary in the large-velocity, highly nonlinear regime, and to witness the final merger of the binary and the excitation of uniquely relativistic modes of the gravitational field. We carry out several investigations to determine whether GW150914 is consistent with a binary black-hole merger in general relativity. We find that the final remnant's mass and spin, as determined from the low-frequency (inspiral) and high-frequency (postinspiral) phases of the signal, are mutually consistent with the binary black-hole solution in general relativity. Furthermore, the data following the peak of GW150914 are consistent with the least-damped quasinormal mode inferred from the mass and spin of the remnant black hole. By using waveform models that allow for parametrized general-relativity violations during the inspiral and merger phases, we perform quantitative tests on the gravitational-wave phase in the dynamical regime and we determine the first empirical bounds on several high-order post-Newtonian coefficients. We constrain the graviton Compton wavelength, assuming that gravitons are dispersed in vacuum in the same way as particles with mass, obtaining a 90%-confidence lower bound of 10^{13} km. In conclusion, within our statistical uncertainties, we find no evidence for violations of general relativity in the genuinely strong-field regime of gravity.

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The record

Venue
Physical Review Letters
Topic
Pulsars and Gravitational Waves Research
Field
Physics and Astronomy
Canadian institutions
Canadian Institute for Theoretical AstrophysicsUniversity of Toronto
Funders
Division of Human Resource DevelopmentAustralian Research CouncilScience and Technology Facilities CouncilIstituto Nazionale di Fisica NucleareNatural Sciences and Engineering Research Council of CanadaMinistry of Science and Technology, TaiwanMinistry of Education, IndiaNarodowe Centrum NaukiNational Research Foundation of KoreaRoyal SocietyMinisterio de Economía y CompetitividadCouncil of Scientific and Industrial Research, IndiaCentre National de la Recherche ScientifiqueIndustry CanadaGovern de les Illes BalearsNederlandse Organisatie voor Wetenschappelijk OnderzoekNational Research FoundationInstituto Nazionale di Fisica NucleareEuropean CommissionRussian Foundation for Basic ResearchCanadian Institute for Advanced ResearchMinistero dello Sviluppo EconomicoInstitut des Origines de LyonLeverhulme TrustScottish Funding CouncilScottish Universities Physics AllianceHungarian Scientific Research FundOntario Ministry of Economic Development and InnovationScience and Engineering Research BoardNational Science FoundationKavli FoundationResearch Corporation for Science Advancement
Keywords
PhysicsTests of general relativityGeneral relativityGravitonLIGOGravitational waveBlack hole (networking)Binary black holeNumerical relativityTheory of relativityQuasinormal modeGravitationClassical mechanicsAstrophysics
Has abstract in OpenAlex
yes