Search for long-lived gravitational-wave transients coincident with long gamma-ray bursts

Zur Kurzanzeige

dc.identifier.uri http://dx.doi.org/10.15488/2134
dc.identifier.uri http://www.repo.uni-hannover.de/handle/123456789/2159
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 2017-10-26T08:40:29Z
dc.date.available 2017-10-26T08:40:29Z
dc.date.issued 2013
dc.identifier.citation Aasi, J.; Abadie, J.; Abbott, B.P.; Abbott, R.; Abbott, T. et al.: Search for long-lived gravitational-wave transients coincident with long gamma-ray bursts. In: Physical Review D - Particles, Fields, Gravitation and Cosmology 88 (2013), Nr. 12, No. 122004. DOI: https://doi.org/10.1103/PhysRevD.88.122004
dc.description.abstract Long gamma-ray bursts (GRBs) have been linked to extreme core-collapse supernovae from massive stars. Gravitational waves (GW) offer a probe of the physics behind long GRBs. We investigate models of long-lived (∼10–1000  s) GW emission associated with the accretion disk of a collapsed star or with its protoneutron star remnant. Using data from LIGO’s fifth science run, and GRB triggers from the Swift experiment, we perform a search for unmodeled long-lived GW transients. Finding no evidence of GW emission, we place 90% confidence-level upper limits on the GW fluence at Earth from long GRBs for three waveforms inspired by a model of GWs from accretion disk instabilities. These limits range from F<3.5  ergs cm−2 to F<1200  ergs cm−2, depending on the GRB and on the model, allowing us to probe optimistic scenarios of GW production out to distances as far as ≈33  Mpc. Advanced detectors are expected to achieve strain sensitivities 10× better than initial LIGO, potentially allowing us to probe the engines of the nearest long GRBs. © 2013 The American Physical Society eng
dc.language.iso eng
dc.publisher College Park, MD : American Physical Society
dc.relation.ispartofseries Physical Review D 88 (2013), Nr. 12
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 long-lived gravitational-wave transients coincident with long gamma-ray bursts
dc.type article
dc.type Text
dc.relation.issn 2470-0010
dc.relation.doi https://doi.org/10.1103/PhysRevD.88.122004
dc.bibliographicCitation.issue 12
dc.bibliographicCitation.volume 88
dc.bibliographicCitation.firstPage 122004
dc.description.version publishedVersion
tib.accessRights frei zug�nglich


Die Publikation erscheint in Sammlung(en):

Zur Kurzanzeige

 

Suche im Repositorium


Durchblättern

Mein Nutzer/innenkonto

Nutzungsstatistiken