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Accès ouvert déclaré 2020 article

Optically targeted search for gravitational waves emitted by core-collapse supernovae during the first and second observing runs of advanced LIGO and advanced Virgo

123Citations signalées, ce qui n’est pas une note de qualité
212Institutions déclarées
29Pays d’affiliation déclarés

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

Le résumé fourni par la source

We present the results from a search for gravitational-wave transients associated with core-collapse supernovae observed within a source distance of approximately 20 Mpc during the first and second observing runs of Advanced LIGO and Advanced Virgo. No significant gravitational-wave candidate was detected. We report the detection efficiencies as a function of the distance for waveforms derived from multidimensional numerical simulations and phenomenological extreme emission models. The sources with neutrino-driven explosions are detectable at the distances approaching 5 kpc, and for magnetorotationally driven explosions the distances are up to 54 kpc. However, waveforms for extreme emission models are detectable up to 28 Mpc. For the first time, the gravitational-wave data enabled us to exclude part of the parameter spaces of two extreme emission models with confidence up to 83%, limited by coincident data coverage. Besides, using ad hoc harmonic signals windowed with Gaussian envelopes, we constrained the gravitational-wave energy emitted during core collapse at the levels of $4.27\ifmmode\times\else\texttimes\fi{}{10}^{\ensuremath{-}4}\text{ }\text{ }{M}_{\ensuremath{\bigodot}}{c}^{2}$ and $1.28\ifmmode\times\else\texttimes\fi{}{10}^{\ensuremath{-}1}\text{ }\text{ }{M}_{\ensuremath{\bigodot}}{c}^{2}$ for emissions at 235 and 1304 Hz, respectively. These constraints are 2 orders of magnitude more stringent than previously derived in the corresponding analysis using initial LIGO, initial Virgo, and GEO 600 data.

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Le contrôle bibliographique ouvert

DOI retrouvé dans Crossref DOI retrouvé ; titre concordant.

Titre Crossref
Optically targeted search for gravitational waves emitted by core-collapse supernovae during the first and second observing runs of advanced LIGO and advanced Virgo
Date Crossref
02/04/2020
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 UniversityInter-University Centre for Astronomy and AstrophysicsUniversity of SalernoIstituto Nazionale di Fisica Nucleare, Sezione di NapoliAustralian Regenerative Medicine InstituteARC Centre of Excellence for Gravitational Wave DiscoveryMonash UniversityLIGO Scientific CollaborationAustralian National UniversityLeibniz University HannoverMax Planck Institute for Gravitational PhysicsUniversity of CambridgeFriedrich Schiller University JenaUniversity of BirminghamMassachusetts Institute of TechnologyInstituto Nacional de Pesquisas EspaciaisIstituto Nazionale di Fisica Nucleare, Laboratori Nazionali del Gran SassoGran Sasso Science InstituteTata Institute of Fundamental ResearchInternational Centre for Theoretical SciencesUniversity of Illinois Urbana-ChampaignUniversity of PisaIstituto Nazionale di Fisica Nucleare, Sezione di PisaUniversitat de ValènciaLaboratoire des Matériaux AvancésUniversity of Wisconsin–MilwaukeeUniversity of StrathclydeDélégation Paris 7Université Paris CitéCalifornia State University, FullertonUniversité Paris-SaclayEuropean Gravitational ObservatoryUniversity of FloridaIstituto Nazionale di Fisica Nucleare, Roma Tor VergataIstituto Nazionale di Fisica Nucleare, Sezione di Roma IUniversité Savoie Mont BlancEmbry–Riddle Aeronautical UniversityMontclair State UniversityNational Institute for Subatomic PhysicsKorea Institute of Science & Technology InformationWest Virginia UniversityUniversity of PerugiaIstituto Nazionale di Fisica Nucleare, Sezione di PerugiaSyracuse UniversityUniversity of MinnesotaUniversity of Minnesota SystemIstituto Nazionale di Fisica Nucleare, Sezione di Milano BicoccaUniversity of Milano-BicoccaUniversity of GlasgowHUN-REN Wigner Research Centre for PhysicsStanford UniversityUniversità di CamerinoUniversity of PaduaIstituto Nazionale di Fisica Nucleare, Sezione di PadovaMontana State UniversityNicolaus Copernicus Astronomical CenterPolish Academy of SciencesThe University of AdelaideNorthwestern UniversityIstituto Nazionale di Fisica Nucleare, Sezione di GenovaRaja Ramanna Centre for Advanced TechnologyLomonosov Moscow State UniversityRochester Institute of TechnologyUniversity of UrbinoIstituto Nazionale di Fisica Nucleare, Sezione di FirenzeUniversité Côte d'AzurObservatoire de la Côte d’AzurThe University of Western AustraliaRadboud University NijmegenIstituto Nazionale di Fisica Nucleare, Gruppo Collegato di SalernoUniversity of ZurichFonctions Optiques pour les Technologies de l’informationUniversity of OregonUniversité Paris Sciences et LettresSorbonne UniversitéLaboratoire MédiationsAstronomical ObservatoryUniversity of WarsawVrije Universiteit AmsterdamUniversity of Maryland, College ParkGeorgia Institute of TechnologyUniversité de LyonGoddard Space Flight CenterUniversity of GenoaThe University of TokyoTsinghua UniversityTexas Tech UniversityUniversity of Rome Tor VergataMissouri University of Science and TechnologyUniversity of MississippiCentro Ricerche Enrico FermiPennsylvania State UniversityNational Tsing Hua UniversityCharles Sturt UniversityUniversity of ChicagoChinese University of Hong KongSeoul National UniversityPusan National UniversityCarleton CollegeOsservatorio Astronomico di PadovaThe University of MelbourneFundació Universitat-Empresa de les Illes BalearsUniversitat de les Illes BalearsUniversité Libre de BruxellesSonoma State UniversityColumbia UniversityCardiff UniversityUniversity of Rhode IslandThe University of Texas Rio Grande ValleyBellevue CollegeEötvös Loránd UniversityInstitute for Plasma ResearchUniversity of SheffieldUniversidade de Santiago de CompostelaUniversity of ParmaUniversity of SannioUniversity of TrentoIstituto Nazionale di Fisica Nucleare, Trento Institute for Fundamental Physics And ApplicationsSapienza University of RomeColorado State UniversityKenyon CollegeChristopher Newport UniversityUniversity of BasilicataNational Astronomical Observatory of JapanIstituto Nazionale di Fisica Nucleare, Sezione di TorinoUniversity of EdinburghIndian Institute of Advanced ResearchIndian Institute of Technology BombayUniversity of SzegedUniversity of the West of ScotlandCalifornia State University SystemCalifornia State University Los AngelesUniversität HamburgPark UniversityAstronomical Observatory of CapodimonteUniversity of MichiganWashington State UniversityAmerican UniversityUniversity of PortsmouthUniversity of California SystemUniversity of California, BerkeleyDelta Institute for Theoretical PhysicsUniversity of AmsterdamResearch & Development Establishment (Engrs.)University of BiałystokUniversity of LondonKing's College LondonUniversidad de LondresUniversity College LondonUniversity of SouthamptonUniversity of Washington BothellInstitute of Applied PhysicsEwha Womans UniversityEwha Womans University Medical CenterInje UniversityNational Institute for Mathematical SciencesUlsan National Institute of Science and TechnologyMaastricht UniversityBard CollegeChennai Mathematical InstituteInstitute of Mathematics and InformaticsCzech Academy of Sciences, Institute of MathematicsInstitute of MathematicsCornell UniversityNational Centre for Nuclear ResearchHillsdale CollegeKorea Astronomy and Space Science InstituteHanyang UniversityMarshall Space Flight CenterRoma Tre UniversityIstituto Nazionale di Fisica Nucleare, Sezione di Roma TreCentre National de la Recherche ScientifiqueESPCI ParisSwinburne University of TechnologySouthern University and Agricultural and Mechanical CollegeScientific Centre of MonacoIndian Institute of Technology MadrasIndian Institute of Science Education and Research KolkataMax Planck Institute for Nuclear PhysicsWhitman CollegeHobart and William Smith CollegesUniversity of TurinUniversity of WashingtonBrera Astronomical ObservatoryUniversity of LisbonMarquette UniversityIndian Institute of Technology GandhinagarPolytechnique MontréalUniversité de MontréalIndian Institute of Technology HyderabadOsservatorio Astrofisico di CataniaOsservatorio di Astrofisica e Scienza dello SpazioNational Institute for AstrophysicsUniversidade Federal do Rio Grande do NorteVillanova UniversityAndrews UniversityUniversity of SienaTrinity UniversityUniversity of GroningenCarnegie ObservatoriesThe Ohio State UniversityMillennium Institute of AstrophysicsUniversidad Diego PortalesUniversity of Hawaii SystemUniversity of Hawaii–West OahuUniversity of North Carolina at Chapel HillPulkovo ObservatoryKitt Peak National ObservatoryStockholm UniversityAlbaNovaUniversity of California, Davis

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

Les sujets associés

Pulsars and Gravitational Waves ResearchGamma-ray bursts and supernovaeAtomic and Subatomic Physics Research

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