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Accès ouvert déclaré 2023 article

Search for subsolar-mass black hole binaries in the second part of Advanced LIGO’s and Advanced Virgo’s third observing run

56Citations signalées, ce qui n’est pas une note de qualité
296Institutions déclarées
25Pays d’affiliation déclarés

Rattachement africain : us, jp, it, au, de, in, gb, br, fr, nl, es, gr, be, kr, hu, pl, ru, il, cn, tw, hk, ca, ch, pt, cz. Niveau de preuve : code pays fourni par la source.

Le résumé fourni par la source

ABSTRACT We describe a search for gravitational waves from compact binaries with at least one component with mass $0.2$–$1.0 \, \mathrm{M}_\odot$ and mass ratio q ≥ 0.1 in Advanced Laser Interferometer Gravitational-Wave Observatory (LIGO) and Advanced Virgo data collected between 2019 November 1, 15:00 utc and 2020 March 27, 17:00 utc. No signals were detected. The most significant candidate has a false alarm rate of $0.2 \, \rm {yr}^{-1}$. We estimate the sensitivity of our search over the entirety of Advanced LIGO’s and Advanced Virgo’s third observing run, and present the most stringent limits to date on the merger rate of binary black holes with at least one subsolar-mass component. We use the upper limits to constrain two fiducial scenarios that could produce subsolar-mass black holes: primordial black holes (PBH) and a model of dissipative dark matter. The PBH model uses recent prescriptions for the merger rate of PBH binaries that include a rate suppression factor to effectively account for PBH early binary disruptions. If the PBHs are monochromatically distributed, we can exclude a dark matter fraction in PBHs $f_\mathrm{PBH} \gtrsim \, 0.6$ (at 90 per cent confidence) in the probed subsolar-mass range. However, if we allow for broad PBH mass distributions, we are unable to rule out fPBH = 1. For the dissipative model, where the dark matter has chemistry that allows a small fraction to cool and collapse into black holes, we find an upper bound fDBH < 10−5 on the fraction of atomic dark matter collapsed into black holes.

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Le contrôle bibliographique ouvert

DOI retrouvé dans Crossref DOI retrouvé ; titre concordant.

Titre Crossref
Search for subsolar-mass black hole binaries in the second part of Advanced LIGO’s and Advanced Virgo’s third observing run
Date Crossref
28/02/2023
Éditeur
Oxford University Press (OUP)
Type
journal-article

Ce recoupement confirme des métadonnées liées au DOI. Il ne confirme ni la méthode ni les conclusions de l’étude, et il ne compte pas comme une seconde source scientifique indépendante.

Les institutions déclarées

California Institute of TechnologyTokyo Institute of TechnologyUniversity of SalernoIstituto Nazionale di Fisica Nucleare, Sezione di NapoliARC Centre of Excellence for Gravitational Wave DiscoveryMonash UniversityPennsylvania State UniversityUniversity of Wisconsin–MilwaukeeLouisiana State UniversityAustralian National UniversityLeibniz University HannoverMax Planck Institute for Gravitational PhysicsInter-University Centre for Astronomy and AstrophysicsUniversity of CambridgeFriedrich Schiller University JenaInstituto Nacional de Pesquisas EspaciaisCardiff UniversityIstituto Nazionale di Fisica Nucleare, Sezione di PisaTata Institute of Fundamental ResearchInternational Centre for Theoretical SciencesNational Astronomical Observatory of JapanIstituto Nazionale di Fisica Nucleare, Sezione di TorinoUniversity of TurinUniversity of GlasgowCentre National de la Recherche ScientifiqueLaboratoire d’Annecy de Physique des ParticulesInstitut National de Physique Nucléaire et de Physique des ParticulesUniversity of Naples Federico IIMaastricht UniversityNational Institute for Subatomic PhysicsThe University of TokyoInstitut Català de Ciències del ClimaUniversitat de BarcelonaInstitució Catalana de Recerca i Estudis AvançatsInstitute for High Energy PhysicsGran Sasso Science InstituteUniversity of UdineIstituto Nazionale di Fisica Nucleare, Sezione di TriesteEmbry–Riddle Aeronautical UniversityUniversité Côte d'AzurAstrophysique Relativiste, Théories, Expériences, Métrologie, Instrumentation, SignauxObservatoire de la Côte d’AzurUniversity of AmsterdamNational and Kapodistrian University of AthensUniversità di CamerinoIstituto Nazionale di Fisica Nucleare, Sezione di PerugiaAmerican UniversityCalifornia State University, FullertonUniversité Paris CitéLaboratoire AstroParticule et CosmologieUniversité Paris-SaclayLaboratoire de Physique des 2 Infinis Irène Joliot-CurieEuropean Gravitational ObservatoryGeorgia Institute of TechnologyChennai Mathematical InstituteHirosaki UniversityRoyal Holloway University of LondonThe Graduate University for Advanced Studies, SOKENDAIUniversity of UrbinoIstituto Nazionale di Fisica Nucleare, Sezione di FirenzeLIGO Scientific CollaborationIstituto Nazionale di Fisica Nucleare, Sezione di Roma IUCLouvainUniversity of LondonKing's College LondonUniversity College LondonKorea Institute of Science & Technology InformationNational Institute for Mathematical SciencesKenyon CollegeUtrecht UniversityUniversity of OregonSyracuse UniversityUniversity of LiègeNorthwestern UniversityMassachusetts Institute of TechnologyHUN-REN Wigner Research Centre for PhysicsUniversity of FloridaStanford UniversityUniversity of PisaUniversity of PerugiaUniversity of PaduaIstituto Nazionale di Fisica Nucleare, Sezione di PadovaMontana State UniversityInstitute for Plasma ResearchGhent UniversityNicolaus Copernicus Astronomical CenterPolish Academy of SciencesUniversity of SannioThe University of AdelaideUniversity of MinnesotaUniversität HamburgUniversity of StrathclydeUniversitat de les Illes BalearsUniversitat Autònoma de BarcelonaIstituto Nazionale di Fisica Nucleare, Sezione di GenovaThe University of Western AustraliaRaja Ramanna Centre for Advanced TechnologyMissouri University of Science and TechnologyVrije Universiteit AmsterdamLomonosov Moscow State UniversityCenter for Theoretical PhysicsUniversity of TrentoIstituto Nazionale di Fisica Nucleare, Trento Institute for Fundamental Physics And ApplicationsBar-Ilan UniversityIstituto Nazionale di Fisica Nucleare, Gruppo Collegato di SalernoSapienza University of RomeFonctions Optiques pour les Technologies de l’informationUniversité de RennesIndian Institute of Technology BombayIstituto Nazionale di Fisica Nucleare, Laboratori Nazionali del Gran SassoCollège de FranceUniversité Paris Sciences et LettresLaboratoire Kastler BrosselÉcole Normale Supérieure - PSLSorbonne UniversitéChristopher Newport UniversityUniversity of BirminghamUniversity of WarsawUniversity of Maryland, College ParkIstituto Nazionale di Fisica Nucleare, Sezione di Milano BicoccaUniversity of Milano-BicoccaUniversité Toulouse III - Paul SabatierUniversité Fédérale de Toulouse Midi-PyrénéesLaboratoire des 2 Infinis ToulouseUniversity of PortsmouthLyon 1 UniversitéInstitut Lumière MatièreUniversidade de Santiago de CompostelaFlatiron Health (United States)Flatiron InstituteStony Brook UniversityGoddard Space Flight CenterUniversity of GenoaBeijing Normal UniversityTexas A&M UniversityThe University of MelbourneUniversity of SassariIstituto Nazionale di Fisica Nucleare, Laboratori Nazionali del SudUniversity of Rome Tor VergataIstituto Nazionale di Fisica Nucleare, Roma Tor VergataUniversitat de ValènciaRochester Institute of TechnologyNational Tsing Hua UniversityChinese University of Hong KongFukuoka UniversityCharles Sturt UniversityTamkang UniversityNational Central UniversityInstitute of Physics, Academia SinicaInstitute of Nuclear Physics of LyonInstitut de Physique des 2 Infinis de LyonOsservatorio Astronomico di PadovaSwinburne University of TechnologyUniversité Libre de BruxellesTexas Tech UniversityUniversity of British ColumbiaColumbia UniversityUniversity of Rhode IslandThe University of Texas Rio Grande ValleyBellevue CollegeScuola Normale SuperioreEötvös Loránd UniversityVillanova UniversityUniversity of SheffieldLaboratoire des Matériaux AvancésUniversity of ParmaUniversity of UtahCarleton CollegeNational Centre for Nuclear ResearchInstitut d'Astrophysique de ParisUniversity of ZurichPerimeter InstituteInstitut Pluridisciplinaire Hubert CurienUniversité de StrasbourgUniversity of ChicagoMontclair State UniversityColorado State UniversityHUN-REN Institute for Nuclear ResearchThe University of Texas at AustinSuperconducting and other Innovative Materials and Devices InstituteUniversity of BasilicataUniversity of MinhoNiigata UniversityOsaka City UniversityVanderbilt UniversityChinese Academy of SciencesWuhan Institute of Physics and MathematicsUniversidad Autónoma de MadridUniversity of the West of ScotlandUniversity of SzegedAstronomical Observatory of CapodimonteQueen Mary University of LondonÉcole Nationale Supérieure d'Ingénieurs de CaenLaboratoire de Physique Corpusculaire de CaenUniversité de Caen NormandieUniversity of MississippiUniversity of MichiganUlsan National Institute of Science and TechnologyShanghai Astronomical ObservatoryKavli Institute for the Physics and Mathematics of the UniverseUniversity of ToyamaUniversity of California, BerkeleyCalifornia State University Los AngelesLancaster UniversityNihon UniversityCollege of Industrial TechnologyRutherford Appleton LaboratoryChungnam National UniversityAoyama Gakuin UniversityPeking UniversityKavli Institute for Theoretical SciencesAristotle University of ThessalonikiResearch & Development Establishment (Engrs.)University of AntwerpUniversity of BiałystokEwha Womans UniversityNational Space Science CenterNational Astronomical ObservatoriesUniversity of Chinese Academy of SciencesUniversity of SouthamptonChung-Ang UniversityUniversity of Washington BothellInstitute of Applied PhysicsInje UniversityMyongji UniversitySungkyunkwan UniversityBard CollegeHigh Energy Accelerator Research OrganizationInstitute of MathematicsNagoya UniversityPolytechnique MontréalUniversité de MontréalLagrange LaboratorySeoul National UniversityLaboratoire Ville Mobilité TransportUniversité Gustave EiffelUniversity of FlorenceNational Cheng Kung UniversityWuhan UniversityNational Institutes of Applied ResearchNational Taiwan Normal UniversityMarshall Space Flight CenterIstituto Nazionale di Fisica Nucleare, Sezione di Roma TreESPCI ParisWest Virginia UniversityTongji UniversityTsinghua UniversityUniversity of TriesteIndian Institute of Technology MadrasInstitute of Space and Astronautical ScienceInstitut des Hautes Études ScientifiquesRyukoku UniversityIndian Institute of Science Education and Research KolkataInstitut de Recherche en Informatique FondamentaleUniversity of Notre DameObservatoire de ParisCentre de Gestion ScientifiqueLaboratoire Univers et ThéoriesJanssen (France)Systèmes de Référence Temps-EspaceCzech Academy of SciencesFZU ‒ Institute of Physics of the Academy of Sciences of the Czech RepublicCornell UniversityInstitute for Complex SystemsKorea Astronomy and Space Science InstituteHobart and William Smith CollegesUniversidade Federal do Rio Grande do NorteCentro Ricerche Enrico FermiRoma Tre UniversityUniversity of California, RiversideUniversity of WashingtonNagaoka National College of TechnologyBrera Astronomical ObservatoryUniversity of AveiroMarquette UniversityToho UniversityIndian Institute of Technology GandhinagarGunma UniversityChapman UniversityOsaka Institute of TechnologyArcetri Astrophysical ObservatoryIndian Institute of Technology HyderabadIndian Institute of Science Education and Research PuneInstitute for Space Astrophysics and PlanetologyAndrews UniversityTokyo City UniversityKyoto UniversityUniversity of GroningenVrije Universiteit BrusselNational Defense Academy of JapanNagaoka University of TechnologyEindhoven University of TechnologySejong UniversityConcordia University WisconsinNational Yang Ming Chiao Tung UniversityRikkyo University

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Les sujets associés

Pulsars and Gravitational Waves ResearchCosmology and Gravitation TheoriesGamma-ray bursts and supernovae

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