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
|
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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 |
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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, 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 |
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dc.relation.ispartofseries |
Physical Review D 88 (2013), Nr. 12 |
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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 |
eng |
dc.type |
Article |
|
dc.type |
Text |
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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 |
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tib.accessRights |
frei zug�nglich |
|