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Accès ouvert déclaré 2016 article

Observing gravitational-wave transient GW150914 with minimal assumptions

203Citations signalées, ce qui n’est pas une note de qualité
138Institutions déclarées
19Pays d’affiliation déclarés

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

Le résumé fourni par la source

The recent announcement by LIGO of the detection of the gravitational-wave signal GW150914 has ignited tremendous interest. The two manuscripts highlighted here detail the impressive analysis performed by LIGO to identify a specific black hole binary merger as the source of GW150914. The papers describe two independent methods of analysis: the matching of the signal to numerical-relativity-generated templates and unmodeled burst analyses. The two papers together provide detailed and virtually incontrovertible evidence, by the standards of experimental physics, of the detection of gravitational waves generated by a merger of a black hole binary system consisting initially of black holes of approximately 36 and 29 solar masses.

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
Observing gravitational-wave transient GW150914 with minimal assumptions
Date Crossref
07/06/2016
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 TechnologyLouisiana State UniversityUniversity of SalernoIstituto Nazionale di Fisica Nucleare, Sezione di NapoliUniversity of FloridaLIGO Scientific CollaborationUniversité Savoie Mont BlancMax Planck Institute for Gravitational PhysicsNational Institute for Subatomic PhysicsMassachusetts Institute of TechnologyInstituto Nacional de Pesquisas EspaciaisIstituto Nazionale di Fisica Nucleare, Roma Tor VergataGran Sasso Science InstituteInter-University Centre for Astronomy and AstrophysicsTata Institute of Fundamental ResearchInternational Centre for Theoretical SciencesLeibniz University HannoverUniversity of Wisconsin–MilwaukeeUniversity of PisaIstituto Nazionale di Fisica Nucleare, Sezione di PisaAustralian National UniversityUniversity of MississippiCalifornia State University, FullertonUniversité Paris-SaclayChennai Mathematical InstituteUniversity of Rome Tor VergataUniversity of SouthamptonUniversität HamburgIstituto Nazionale di Fisica Nucleare, Sezione di Roma IDélégation Paris 7Université Paris CitéMontana State UniversityUniversity of PerugiaIstituto Nazionale di Fisica Nucleare, Sezione di PerugiaEuropean Gravitational ObservatorySyracuse UniversityUniversity of GlasgowHUN-REN Wigner Research Centre for PhysicsColumbia UniversityStanford UniversityUniversity of PaduaIstituto Nazionale di Fisica Nucleare, Sezione di PadovaUniversity of BirminghamIstituto Nazionale di Fisica Nucleare, Sezione di GenovaUniversity of GenoaRaja Ramanna Centre for Advanced TechnologyLomonosov Moscow State UniversityUniversity of the West of ScotlandThe University of Western AustraliaRadboud University NijmegenUniversité Côte d'AzurObservatoire de la Côte d’AzurEötvös Loránd UniversityUniversité de RennesWashington State UniversityUniversity of UrbinoIstituto Nazionale di Fisica Nucleare, Sezione di FirenzeUniversity of OregonUniversité Paris Sciences et LettresÉcole Normale Supérieure - PSLAstronomical ObservatoryUniversity of WarsawVrije Universiteit AmsterdamUniversity of Maryland, College ParkGeorgia Institute of TechnologyLyon 1 UniversitéUniversité de LyonFundació Universitat-Empresa de les Illes BalearsUniversitat de les Illes BalearsGoddard Space Flight CenterUniversity of TorontoCanadian Institute for Theoretical AstrophysicsTsinghua UniversityTexas Tech UniversityPennsylvania State UniversityNational Tsing Hua UniversityCharles Sturt UniversityUniversity of ChicagoKorea Institute of Science & Technology InformationCarleton CollegeSapienza University of RomeSonoma State UniversityNorthwestern UniversityUniversity of MinnesotaUniversity of Minnesota SystemThe University of MelbourneThe University of Texas Rio Grande ValleyUniversity of SheffieldUniversity of SannioMontclair State UniversityUniversity of TrentoIstituto Nazionale di Fisica Nucleare, Trento Institute for Fundamental Physics And ApplicationsCardiff UniversityNational Astronomical Observatory of JapanUniversity of EdinburghIndian Institute of Technology GandhinagarInstitute for Plasma ResearchUniversity of SzegedEmbry–Riddle Aeronautical UniversityUniversity of MichiganAmerican UniversityRochester Institute of TechnologyUniversity of Massachusetts AmherstThe University of AdelaideWest Virginia UniversityUniversity of BiałystokUniversity of StrathclydeIndian Institute of Science Education and Research ThiruvananthapuramInstitute of Applied PhysicsPusan National UniversityHanyang UniversityInstitute of MathematicsNational Centre for Nuclear ResearchAustralian Regenerative Medicine InstituteMonash UniversitySeoul National UniversityUniversity of Alabama in HuntsvilleCentre National de la Recherche ScientifiqueESPCI ParisUniversità di CamerinoSouthern University and Agricultural and Mechanical CollegeWilliam & MaryWilliams (United States)American Institute for Economic ResearchICTP South American Institute for Fundamental ResearchUniversity of CambridgeIndian Institute of Science Education and Research KolkataRutherford Appleton LaboratoryWhitman CollegeNational Institute for Mathematical SciencesHobart and William Smith CollegesUniversity of Zielona GóraAndrews UniversityUniversity of SienaTrinity UniversityUniversity of WashingtonKenyon CollegeAbilene Christian University

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

Les sujets associés

Pulsars and Gravitational Waves ResearchHigh-pressure geophysics and materialsGamma-ray bursts and supernovae

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