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Record W3167754487

[no title]

2021· article· ca· W3167754487 on OpenAlexfundno aff
R. Abbott, T. D. Abbott, S. Abraham, F. Acernese, K. Ackley, A. Adams, C. Adams, R. X. Adhikari, V. B. Adya, C. Affeldt, D. Agarwal, M. Agathos, K. Agatsuma, N. Aggarwal, O. D. Aguiar, L. Aiello, A. Ain, P. Ajith, T. Akutsu, K. M. Aleman, B. Allen, A. Allocca, P. A. Altin, A. Amato, Shreya Anand, A. Ananyeva, S. B. Anderson, W. G. Anderson, Masaki Ando, S. V. Angelova, S. Ansoldi, Javier M. Antelis, S. Antier, S. Appert, Koya Arai, Koji Arai, Y. Arai, S. Araki, A. Araya, M. C. Araya, J. S. Areeda, M. Arène, N. Aritomi, N. Arnaud, K. G. Arun, Hideki Asada, Y. Asali, G. Ashton, Y. Aso, S. M. Aston, P. Astone, F. Aubin, P. Aufmuth, K. AultONeal, C. Austin, S. Babak, F. Badaracco, M. K. M. Bader, S. Bae, Y. Bae, A. M. Baer, S. Bagnasco, Y. Bai, Luca Baiotti, J. Baird, R. Bajpai, M. Ball, G. Ballardin, S. W. Ballmer, M. Bals, A. Balsamo, G. Baltus, S. Banagiri, D. Bankar, R. S. Bankar, J. C. Barayoga, C. Barbieri, B. C. Barish, D. Barker, P. Barneo, S. Barnum, F. Barone, B. Barr, L. Barsotti, M. Barsuglia, D. Barta, J. Bartlett, M. A. Barton, I. Bartos, R. Bassiri, M. Bawaj, J. C. Bayley, A. C. Baylor, M. Bazzan, B. Bécsy, V. M. Bedakihale, M. Bejger, I. Belahcene

Bibliographic record

VenueLancaster EPrints (Lancaster University) · 2021
Typearticle
Languageca
FieldPhysics and Astronomy
TopicPulsars and Gravitational Waves Research
Canadian institutionsnot available
FundersAstrophysics DivisionAstrophysics Science DivisionNational Research, Development and Innovation OfficeJapan Society for the Promotion of ScienceSchweizerischer Nationalfonds zur Förderung der Wissenschaftlichen ForschungScience and Technology Facilities CouncilSmithsonian Astrophysical ObservatoryGoddard Space Flight CenterEuropean Regional Development FundCentre National de la Recherche ScientifiqueICTP South American Institute for Fundamental ResearchNational Astronomical Observatory of JapanMinistry of Education, IndiaConseil Régional, Île-de-FranceScottish Universities Physics AllianceNational Natural Science Foundation of ChinaNational Research Foundation of KoreaNuclear Safety and Security CommissionLeverhulme TrustEuropean CommissionEngineering and Physical Sciences Research CouncilHungarian Scientific Research FundGeneralitat de CatalunyaGeneralitat ValencianaInstitut des Origines de LyonCentres de Recerca de CatalunyaNational Aeronautics and Space AdministrationIndustry CanadaIstituto Nazionale di Fisica NucleareSmithsonian InstitutionGreat Southern Development Commission, Government of Western AustraliaAgencia Estatal de InvestigaciónGovern de les Illes BalearsKorea Institute of Science and Technology InformationMinistry of Education, Culture, Sports, Science and TechnologyInstitute for Cosmic Ray Research, University of TokyoCouncil of Scientific and Industrial Research, IndiaVlaamse regeringNemzeti Kutatási Fejlesztési és Innovációs HivatalNational Research FoundationAcademia SinicaAbdus Salam International Centre for Theoretical PhysicsFonds De La Recherche Scientifique - FNRSRussian Foundation for Basic ResearchRussian Science FoundationScottish Funding CouncilDivision of Human Resource DevelopmentMinistero dello Sviluppo EconomicoUniversidad de Santiago de ChileFonds Wetenschappelijk OnderzoekScience and Engineering Research BoardNational Science Foundation
KeywordsPhysicsLIGOGravitational wavePulsarEphemerisAstrophysicsNeutron starAstronomyLuminosityGravitational-wave observatoryRotation (mathematics)SatelliteGalaxy
DOInot available

Abstract

fetched live from OpenAlex

We present a search for continuous gravitational-wave signals from the young, energetic X-ray pulsar PSR J0537-6910 using data from the second and third observing runs of LIGO and Virgo. The search is enabled by a contemporaneous timing ephemeris obtained using NICER data. The NICER ephemeris has also been extended through 2020 October and includes three new glitches. PSR J0537-6910 has the largest spin-down luminosity of any pulsar and is highly active with regards to glitches. Analyses of its long-term and inter-glitch braking indices provided intriguing evidence that its spin-down energy budget may include gravitational-wave emission from a time-varying mass quadrupole moment. Its 62 Hz rotation frequency also puts its possible gravitational-wave emission in the most sensitive band of LIGO/Virgo detectors. Motivated by these considerations, we search for gravitational-wave emission at both once and twice the rotation frequency. We find no signal, however, and report our upper limits. Assuming a rigidly rotating triaxial star, our constraints reach below the gravitational-wave spin-down limit for this star for the first time by more than a factor of two and limit gravitational waves from the $l=m=2$ mode to account for less than 14% of the spin-down energy budget. The fiducial equatorial ellipticity is limited to less than about 3e-5, which is the third best constraint for any young pulsar.

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 categoriesMeta-epidemiology (narrow), Insufficient payload (model declined to judge)
Consensus categoriesInsufficient payload (model declined to judge)
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Observational · Consensus signal: Observational
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.296
Threshold uncertainty score0.999

Codex and Gemma teacher scores by category

CategoryCodexGemma
Metaresearch0.0000.000
Meta-epidemiology (narrow)0.0010.001
Meta-epidemiology (broad)0.0010.001
Bibliometrics0.0010.003
Science and technology studies0.0010.000
Scholarly communication0.0010.002
Open science0.0020.003
Research integrity0.0000.002
Insufficient payload (model declined to judge)0.0050.003

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 head0.016
GPT teacher head0.277
Teacher spread0.261 · 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; both teacher heads agree on what is shown here.

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

Citations43
Published2021
Admission routes1
Has abstractyes

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