Search for gravitational waves associated with γ-ray bursts detected by the interplanetary network

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dc.identifier.uri http://dx.doi.org/10.15488/2129
dc.identifier.uri http://www.repo.uni-hannover.de/handle/123456789/2154
dc.contributor.author Aasi, J.
dc.contributor.author Allen, Bruce
dc.contributor.author Ast, Stefan
dc.contributor.author Aufmuth, Peter
dc.contributor.author Danzmann, Karsten
dc.contributor.author Kaufer, S.
dc.contributor.author Lück, Harald
dc.contributor.author Meier, Tobias
dc.contributor.author Schnabel, R.
dc.contributor.author Vahlbruch, H.
dc.contributor.author Willke, Benno
dc.contributor.author et al.
dc.contributor.author LIGO Scientific Collaboration
dc.contributor.author Virgo Collaboration
dc.date.accessioned 2017-10-26T08:40:27Z
dc.date.available 2017-10-26T08:40:27Z
dc.date.issued 2014
dc.identifier.citation Aasi, J.; Abbott, B.P.; Abbott, R.; Abbott, T.; Abernathy, M.R. et al.: Search for gravitational waves associated with γ-ray bursts detected by the interplanetary network. In: Physical Review Letters 113 (2014), Nr. 1, No. 11102. DOI: https://doi.org/10.1103/PhysRevLett.113.011102
dc.description.abstract We present the results of a search for gravitational waves associated with 223 γ-ray bursts (GRBs) detected by the InterPlanetary Network (IPN) in 2005–2010 during LIGO’s fifth and sixth science runs and Virgo’s first, second, and third science runs. The IPN satellites provide accurate times of the bursts and sky localizations that vary significantly from degree scale to hundreds of square degrees. We search for both a well-modeled binary coalescence signal, the favored progenitor model for short GRBs, and for generic, unmodeled gravitational wave bursts. Both searches use the event time and sky localization to improve the gravitational wave search sensitivity as compared to corresponding all-time, all-sky searches. We find no evidence of a gravitational wave signal associated with any of the IPN GRBs in the sample, nor do we find evidence for a population of weak gravitational wave signals associated with the GRBs. For all IPN-detected GRBs, for which a sufficient duration of quality gravitational wave data are available, we place lower bounds on the distance to the source in accordance with an optimistic assumption of gravitational wave emission energy of 10−2M⊙c2 at 150 Hz, and find a median of 13 Mpc. For the 27 short-hard GRBs we place 90% confidence exclusion distances to two source models: a binary neutron star coalescence, with a median distance of 12 Mpc, or the coalescence of a neutron star and black hole, with a median distance of 22 Mpc. Finally, we combine this search with previously published results to provide a population statement for GRB searches in first-generation LIGO and Virgo gravitational wave detectors and a resulting examination of prospects for the advanced gravitational wave detectors. © 2014 The American Physical Society eng
dc.language.iso eng
dc.publisher College Park, MD : American Physical Society
dc.relation.ispartofseries Physical Review Letters 113 (2014), Nr. 1
dc.rights Es gilt deutsches Urheberrecht. Das Dokument darf zum eigenen Gebrauch kostenfrei genutzt, aber nicht im Internet bereitgestellt oder an Außenstehende weitergegeben werden.
dc.subject Gravitational waves eng
dc.subject Gamma-Ray Bursts eng
dc.subject Gravitationswelle ger
dc.subject.ddc 530 | Physik ger
dc.title Search for gravitational waves associated with γ-ray bursts detected by the interplanetary network eng
dc.type article
dc.type Text
dc.relation.issn 0031-9007
dc.relation.doi https://doi.org/10.1103/PhysRevLett.113.011102
dc.bibliographicCitation.issue 1
dc.bibliographicCitation.volume 113
dc.bibliographicCitation.firstPage 11102
dc.description.version publishedVersion
tib.accessRights frei zug�nglich


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