Aller au contenu principal
Accès ouvert déclaré 2013 article

Search for gravitational waves from binary black hole inspiral, merger, and ringdown in LIGO-Virgo data from 2009–2010

119Citations signalées, ce qui n’est pas une note de qualité
116Institutions déclarées
18Pays d’affiliation déclarés

Rattachement africain : us, gb, fr, it, de, nl, jp, ru, au, pl, es, ca, cn, kr, br, hu, in, se. Niveau de preuve : code pays fourni par la source.

Le résumé fourni par la source

We report a search for gravitational waves from the inspiral, merger and ringdown of binary black holes (BBH) with total mass between 25 and 100 solar masses, in data taken at the LIGO and Virgo observatories between July 7, 2009 and October 20, 2010. The maximum sensitive distance of the detectors over this period for a $(20,20){\mathrm{M}}_{\ensuremath{\bigodot}}$ coalescence was 300 Mpc. No gravitational wave signals were found. We thus report upper limits on the astrophysical coalescence rates of BBH as a function of the component masses for nonspinning components, and also evaluate the dependence of the search sensitivity on component spins aligned with the orbital angular momentum. We find an upper limit at 90% confidence on the coalescence rate of BBH with nonspinning components of mass between 19 and $28{\mathrm{M}}_{\ensuremath{\bigodot}}$ of $3.3\ifmmode\times\else\texttimes\fi{}{10}^{\ensuremath{-}7}$ mergers ${\mathrm{Mpc}}^{\ensuremath{-}3}\text{ }{\mathrm{yr}}^{\ensuremath{-}1}$.

Ce résumé expose les affirmations des auteurs. BNTIC ne l’interprète pas comme une validation indépendante des résultats.

Le contrôle bibliographique ouvert

DOI retrouvé dans Crossref DOI retrouvé ; titre concordant.

Titre Crossref
Search for gravitational waves from binary black hole inspiral, merger, and ringdown in LIGO-Virgo data from 2009–2010
Date Crossref
23/01/2013
Éditeur
American Physical Society (APS)
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 TechnologyCalifornia State University, FullertonUniversity of GlasgowCentre National de la Recherche ScientifiqueLaboratoire d’Annecy de Physique des ParticulesInstitut National de Physique Nucléaire et de Physique des ParticulesUniversity of SalernoIstituto Nazionale di Fisica Nucleare, Sezione di NapoliLIGO Scientific CollaborationCardiff UniversityLeibniz University HannoverMax Planck Institute for Gravitational PhysicsNational Institute for Subatomic PhysicsNational Astronomical Observatory of JapanUniversity of Wisconsin–MilwaukeeUniversity of SienaIstituto Nazionale di Fisica Nucleare, Sezione di PisaUniversity of FloridaIstituto Nazionale di Fisica Nucleare, Sezione di Roma IUniversity of BirminghamMontana State UniversityEuropean Gravitational ObservatorySyracuse UniversityMassachusetts Institute of TechnologyDélégation Paris 7Université Paris CitéCommissariat à l'Énergie Atomique et aux Énergies AlternativesLaboratoire AstroParticule et CosmologieSorbonne Paris CitéColumbia UniversityStanford UniversityUniversity of PisaBrownsville Public LibrarySan Jose State UniversityLomonosov Moscow State UniversityUniversité Paris-SudGoddard Space Flight CenterThe University of Western AustraliaPennsylvania State UniversityInstitut de Physique de RennesUniversité de RennesLaboratoire des Matériaux AvancésWashington State UniversityIstituto Nazionale di Fisica Nucleare, Sezione di PerugiaUniversity of UrbinoIstituto Nazionale di Fisica Nucleare, Sezione di FirenzeUniversity of OregonLaboratoire Kastler BrosselSorbonne UniversitéObservatoire de la Côte d’AzurUniversity of WarsawVrije Universiteit AmsterdamUniversity of Maryland, College ParkUniversitat de les Illes BalearsUniversity of Massachusetts AmherstUniversity of TorontoCanadian Institute for Theoretical AstrophysicsTsinghua UniversityUniversity of MichiganLouisiana State UniversityUniversity of MississippiCharles Sturt UniversityIstituto Nazionale di Fisica Nucleare, Sezione di GenovaPusan National UniversityAustralian National UniversityCarleton CollegeThe University of MelbourneUniversity of Rome Tor VergataIstituto Nazionale di Fisica Nucleare, Roma Tor VergataSapienza University of RomeInstituto Nacional de Pesquisas EspaciaisUniversity of SheffieldHUN-REN Wigner Research Centre for PhysicsInter-University Centre for Astronomy and AstrophysicsUniversity of L'AquilaUniversity of MinnesotaUniversity of TrentoNorthwestern UniversityRochester Institute of TechnologyEötvös Loránd UniversityUniversity of CambridgeUniversity of PerugiaUniversity of SzegedRutherford Appleton LaboratoryEmbry–Riddle Aeronautical UniversityPerimeter InstituteAmerican UniversityUniversity of New HampshireUniversity of BiałystokUniversity of SouthamptonKorea Institute of Science & Technology InformationHobart and William Smith CollegesInstitute of Applied PhysicsLund UniversityHanyang UniversityNational Centre for Nuclear ResearchInstitute of MathematicsSeoul National UniversityUniversity of StrathclydeESPCI ParisUniversità di CamerinoThe University of Texas at AustinSouthern University and Agricultural and Mechanical CollegeUniversity of RochesterThe University of AdelaideNational Institute for Mathematical SciencesUniversity of SannioLouisiana Tech UniversityUniversity of Zielona GóraMcNeese State UniversityAndrews UniversityIstituto Nazionale di Fisica Nucleare, Sezione di PadovaTrinity UniversityUniversity of WashingtonUniversity of PaduaSoutheastern Louisiana University

Une affiliation ne permet pas de déduire la nationalité d’un auteur.

Les sujets associés

Pulsars and Gravitational Waves ResearchAstrophysical Phenomena and ObservationsCosmology and Gravitation Theories

BNTIC News n’est pas le producteur de ces données. Les publications sont interrogées à la demande dans Crossref, OpenAIRE, DOAJ, Europe PMC, HAL, DataCite, AfricArXiv, ROR et la Banque mondiale, sans clé d’accès. OpenAlex reste optionnel. Aucun service payant n’est nécessaire et aucune donnée externe n’est enregistrée en base. Consulter les sources et leurs limites.