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Record W6995825896

Properties and Astrophysical Implications of the 150 M⊙ Binary Black Hole Merger GW190521

2020· article· en· W6995825896 on OpenAlexfundno aff

Bibliographic record

VenueLancaster EPrints (Lancaster University) · 2020
Typearticle
Languageen
FieldPhysics and Astronomy
TopicPulsars and Gravitational Waves Research
Canadian institutionsnot available
FundersDivision of Human Resource DevelopmentScience and Technology Facilities CouncilGovern de les Illes BalearsICTP South American Institute for Fundamental ResearchVlaamse regeringMinistry of Education, IndiaNational Research Foundation of KoreaHungarian Scientific Research FundGeneralitat ValencianaFonds Wetenschappelijk OnderzoekCouncil of Scientific and Industrial Research, IndiaCentre National de la Recherche ScientifiqueCentres de Recerca de CatalunyaIndustry CanadaIstituto Nazionale di Fisica NucleareGeneralitat de CatalunyaNational Natural Science Foundation of ChinaEuropean CommissionNemzeti Kutatási Fejlesztési és Innovációs HivatalAbdus Salam International Centre for Theoretical PhysicsNational Research FoundationFonds De La Recherche Scientifique - FNRSRussian Foundation for Basic ResearchRussian Science FoundationLeverhulme TrustScottish Funding CouncilMinistero dello Sviluppo EconomicoInstitut des Origines de LyonEuropean Regional Development FundScottish Universities Physics AllianceConseil Régional, Île-de-FranceNational Research, Development and Innovation OfficeAgencia Estatal de InvestigaciónSchweizerischer Nationalfonds zur Förderung der Wissenschaftlichen ForschungScience and Engineering Research BoardNational Science Foundation
KeywordsBinary black holeBlack hole (networking)Stellar black holeIntermediate-mass black holeRedshiftBinary numberSpin-flipGeneral relativitySupernova
DOInot available

Abstract

fetched live from OpenAlex

The gravitational-wave signal GW190521 is consistent with a binary black hole merger source at redshift 0.8 with unusually high component masses, 85 +21 -14 M and 66 +17 -18 M , compared to previously reported events, and shows mild evidence for spin-induced orbital precession.The primary falls in the mass gap predicted by (pulsational) pair-instability supernova theory, in the approximate range 65-120 M .The probability that at least one of the black holes in GW190521 is in that range is 99.0%.The final mass of the merger (142 +28 -16 M ) classifies it as an intermediate-mass black hole.Under the assumption of a quasi-circular binary black hole coalescence, we detail the physical properties of GW190521's source binary and its post-merger remnant, including component masses and spin vectors.Three different waveform models, as well as direct comparison to numerical solutions of general relativity, yield consistent estimates of these properties.Tests of strong-field general relativity targeting the merger-ringdown stages of the coalescence indicate consistency of the observed signal with theoretical predictions.We estimate the merger rate of similar systems to be 0.13 +0.30 -0.11 Gpc -3 yr -1 .We discuss the astrophysical implications of GW190521 for stellar collapse, and for the possible formation of black holes in the pair-instability mass gap through various channels: via (multiple) stellar coalescences, or via hierarchical mergers of lower-mass black holes in star clusters or in active galactic nuclei.We find it to be unlikely that GW190521 is a strongly lensed signal of a lower-mass black hole binary merger.We also discuss more exotic possible sources for GW190521, including a highly eccentric black hole binary, or a primordial black hole binary.

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.

How this classification was reachedexpand

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 categoriesnone
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Observational · Consensus signal: Observational
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.328
Threshold uncertainty score0.358

Codex and Gemma teacher scores by category

CategoryCodexGemma
Metaresearch0.0000.000
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0000.000
Science and technology studies0.0000.000
Scholarly communication0.0000.000
Open science0.0000.000
Research integrity0.0000.000
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 head0.034
GPT teacher head0.249
Teacher spread0.215 · 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

Classification

machine, unvalidated

Machine predicted; a candidate call from one teacher head, not a consensus.

The models applied no category: nothing in the taxonomy fit this work.
Study designObservational
Domainnot available
GenreEmpirical

How this classification was reached, model by model and score by score, is at the end of the page under "How this classification was reached".

Quick stats

Citations0
Published2020
Admission routes1
Has abstractyes

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