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Record W3017872349 · doi:10.1103/physrevd.102.043015

GW190412: Observation of a binary-black-hole coalescence with asymmetric masses

2020· article· en· W3017872349 on OpenAlex

Why this work is in the frame

A frame that forgets how it found something cannot be audited. These are the routes that admitted this work.

affAt least one author lists a Canadian institution in the pinned OpenAlex snapshot.
fundA Canadian funder is recorded on the work.

Bibliographic record

VenuePhysical review. D/Physical review. D. · 2020
Typearticle
Languageen
FieldPhysics and Astronomy
TopicPulsars and Gravitational Waves Research
Canadian institutionsUniversité de MontréalPolytechnique Montréal
FundersNational Research, Development and Innovation OfficeAustralian Research CouncilSchweizerischer Nationalfonds zur Förderung der Wissenschaftlichen ForschungMinistério da Ciência, Tecnologia e InovaçãoScience and Technology Facilities CouncilSeventh Framework ProgrammeNemzeti Kutatási Fejlesztési és Innovációs HivatalNational Research FoundationVlaamse regeringNatural Sciences and Engineering Research Council of CanadaMinistry of Education, IndiaConseil Régional, Île-de-FranceFonds De La Recherche Scientifique - FNRSNarodowe Centrum NaukiScottish Universities Physics AllianceNational Natural Science Foundation of ChinaNational Research Foundation of KoreaHungarian Scientific Research FundGeneralitat de CatalunyaGeneralitat ValencianaFonds Wetenschappelijk OnderzoekInstitut des Origines de LyonCentres de Recerca de CatalunyaIndustry CanadaIstituto Nazionale di Fisica NucleareDepartment of Science and Technology, Ministry of Science and Technology, IndiaKavli FoundationAgence Nationale de la RechercheEuropean Regional Development FundICTP South American Institute for Fundamental ResearchCentre National de la Recherche ScientifiqueCouncil of Scientific and Industrial Research, IndiaAbdus Salam International Centre for Theoretical PhysicsInstituto Nazionale di Fisica NucleareLeverhulme TrustEuropean CommissionConselleria de Innovación, Universidades, Ciencia y Sociedad Digital, Generalitat ValencianaRussian Foundation for Basic ResearchCanadian Institute for Advanced ResearchDivision of Human Resource DevelopmentMinistero dello Sviluppo EconomicoRussian Science FoundationScottish Funding CouncilAgencia Estatal de InvestigaciónGovern de les Illes BalearsNederlandse Organisatie voor Wetenschappelijk OnderzoekMinistry of Science and Technology of the People's Republic of ChinaOntario Ministry of Economic Development and InnovationRoyal SocietyScience and Engineering Research BoardNational Science Foundation
KeywordsPhysicsGravitational waveBlack hole (networking)Binary black holeLIGOAstrophysicsDimensionless quantityPopulationBinary numberNumerical relativityRotating black holeGeneral relativityAstronomyClassical mechanicsQuantum mechanicsAccretion (finance)

Abstract

fetched live from OpenAlex

We report the observation of gravitational waves from a binary-black-hole coalescence during the first two weeks of LIGO’s and Virgo’s third observing run. The signal was recorded on April 12, 2019 at 05∶30∶44 UTC with a network signal-to-noise ratio of 19. The binary is different from observations during the first two observing runs most notably due to its asymmetric masses: a <a:math xmlns:a="http://www.w3.org/1998/Math/MathML" display="inline"><a:mo>∼</a:mo><a:mn>30</a:mn><a:mtext> </a:mtext><a:mtext> </a:mtext><a:msub><a:mi>M</a:mi><a:mo stretchy="false">⊙</a:mo></a:msub></a:math> black hole merged with a <d:math xmlns:d="http://www.w3.org/1998/Math/MathML" display="inline"><d:mo>∼</d:mo><d:mn>8</d:mn><d:mtext> </d:mtext><d:mtext> </d:mtext><d:msub><d:mi>M</d:mi><d:mo stretchy="false">⊙</d:mo></d:msub></d:math> black hole companion. The more massive black hole rotated with a dimensionless spin magnitude between 0.22 and 0.60 (90% probability). Asymmetric systems are predicted to emit gravitational waves with stronger contributions from higher multipoles, and indeed we find strong evidence for gravitational radiation beyond the leading quadrupolar order in the observed signal. A suite of tests performed on GW190412 indicates consistency with Einstein’s general theory of relativity. While the mass ratio of this system differs from all previous detections, we show that it is consistent with the population model of stellar binary black holes inferred from the first two observing runs. Published by the American Physical Society 2020

Fetched live from OpenAlex and de-inverted. Abstracts are not stored in this database: the inverted indexes are 8.6 GB of the frame’s 9.3 GB of text, and the host has 13 GB free.

Full frame distilled prediction

Teacher imitation

Not calibrated prevalence, not ground truth. Human validation pending. Learned from the 10,348 direct Codex labels and 10,348 direct Gemma labels. Candidate is the union of thresholded teacher heads; consensus is their intersection. These outputs are machine_predicted_unvalidated and are not human labels or direct frontier model labels.

metaresearch head score (Codex)0.000
metaresearch head score (Gemma)0.000
Version: codex-gemma-dda1882f352aValidation status: machine_predicted_unvalidated
Candidate categoriesMeta-epidemiology (narrow)
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Theoretical or conceptual · Consensus signal: none
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.311
Threshold uncertainty score1.000

Codex and Gemma teacher scores by category

CategoryCodexGemma
Metaresearch0.0000.000
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0010.001
Bibliometrics0.0000.002
Science and technology studies0.0000.000
Scholarly communication0.0000.000
Open science0.0010.000
Research integrity0.0000.001
Insufficient payload (model declined to judge)0.0000.000

Machine scores (provisional)

The two teacher heads of the student model, read on this work. A score orders the frame for review; it never asserts a category, and the validation status ships verbatim with every row.

Baseline scores from an immature model (maturity gate not passed, 7 training rounds). Scores rank; they never assert a category.

Opus teacher head0.033
GPT teacher head0.447
Teacher spread0.415 · how far apart the two teachers sit on this one work
Validation statusscore_only:v0-immature-baseline · verbatim from the scoring run: score_only means the number may rank works, and no category label ships from it