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| dc.identifier.uri | http://dx.doi.org/10.15488/2142 | |
| dc.identifier.uri | http://www.repo.uni-hannover.de/handle/123456789/2167 | |
| dc.contributor.author | Abadie, J.
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| dc.contributor.author | Affeldt, Christoph
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| dc.contributor.author | Allen, Bruce
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| dc.contributor.author | Aufmuth, Peter
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| dc.contributor.author | Aulbert, C.
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| dc.contributor.author | Ballardin, G.
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| dc.contributor.author | Bauchrowitz, J.
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| dc.contributor.author | Bertolini, A.
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| dc.contributor.author | Bock, O.
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| dc.contributor.author | Bogan, C.
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| dc.contributor.author | Born, Michael
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| dc.contributor.author | Breyer, J.
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| dc.contributor.author | Brinkmann, M.
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| dc.contributor.author | Britzger, M.
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| dc.contributor.author | Dahl, K.
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| dc.contributor.author | Danzmann, Karsten
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| dc.contributor.author | Di Palma, Irene
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| dc.contributor.author | Eberle, Tobias
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| dc.contributor.author | Fehrmann, H.
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| dc.contributor.author | Frede, M.
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| dc.contributor.author | Friedrich, Daniel
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| dc.contributor.author | Goetz, E.
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| dc.contributor.author | Goßler, S.
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| dc.contributor.author | Graef, C.
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| dc.contributor.author | Grote, Hartmut
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| dc.contributor.author | Hewitson, M.
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| dc.contributor.author | Kaufer, Henning
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| dc.contributor.author | Kawazoe, F.
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| dc.contributor.author | Khalaidovski, Alexander
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| dc.contributor.author | Kim, H.
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| dc.contributor.author | Kranz, O.
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| dc.contributor.author | Kringel, V.
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| dc.contributor.author | Kühn, G.
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| dc.contributor.author | Kwee, P.
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| dc.contributor.author | Lastzka, N.
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| dc.contributor.author | Leong, J.R.
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| dc.contributor.author | Lück, Harald
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| dc.contributor.author | Machenschalk, Bernd
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| dc.contributor.author | Mazzolo, G.
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| dc.contributor.author | Mehmet, Moritz
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| dc.contributor.author | Meier, Tobias
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| dc.contributor.author | Mossavi, K.
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| dc.contributor.author | Müller-Ebhard, H.
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| dc.contributor.author | Pickenpack, M.
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| dc.contributor.author | Pletsch, H.J.
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| dc.contributor.author | Pöld, J.
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| dc.contributor.author | Prijatelj, M.
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| dc.contributor.author | Prix, R
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| dc.contributor.author | Puncken, O.
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| dc.contributor.author | Röver, C.
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| dc.contributor.author | Rüdiger, A.
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| dc.contributor.author | Salemi, F.
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| dc.contributor.author | Schilling, R.
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| dc.contributor.author | Schnabel, Roman
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| dc.contributor.author | Schreiber, E.
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| dc.contributor.author | Schulz, B.
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| dc.contributor.author | Shaltev, M.
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| dc.contributor.author | Steinlechner, J.
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| dc.contributor.author | Steinlechner, S.
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| dc.contributor.author | Tarabrin, S.P.
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| dc.contributor.author | Taylor, J.R.
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| dc.contributor.author | Thüring, A.
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| dc.contributor.author | Vahlbruch, H.
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| dc.contributor.author | Veltkamp, C.
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| dc.contributor.author | Wanner, A.
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| dc.contributor.author | Weinert, M.
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| dc.contributor.author | Wessels, P.
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| dc.contributor.author | Westphal, Tobias
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| dc.contributor.author | Wette, K.
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| dc.contributor.author | Willke, Benno
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| dc.contributor.author | Winkelmann, L.
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| dc.contributor.author | Winkler, W.
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| dc.contributor.author | Wittel, H.
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| dc.contributor.author | Yamamoto, K.
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| dc.contributor.author | et al.
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| dc.contributor.author | LIGO Scientific Collaboration
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| dc.contributor.author | Virgo Collaboration
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| dc.date.accessioned | 2017-10-26T08:57:11Z | |
| dc.date.available | 2017-10-26T08:57:11Z | |
| dc.date.issued | 2012 | |
| dc.identifier.citation | Abadie, J.; Abbott, B.P.; Abbott, R.; Abbott, T.D.; Abernathy, M. et al.: Upper limits on a stochastic gravitational-wave background using LIGO and Virgo interferometers at 600-1000 Hz. In: Physical Review D - Particles, Fields, Gravitation and Cosmology 85 (2012), Nr. 12, 122001. DOI: https://doi.org/10.1103/PhysRevD.85.122001 | |
| dc.description.abstract | A stochastic background of gravitational waves is expected to arise from a superposition of many incoherent sources of gravitational waves, of either cosmological or astrophysical origin. This background is a target for the current generation of ground-based detectors. In this article we present the first joint search for a stochastic background using data from the LIGO and Virgo interferometers. In a frequency band of 600–1000 Hz, we obtained a 95% upper limit on the amplitude of ΩGW(f)=Ω3(f/900 Hz)3, of Ω3<0.32, assuming a value of the Hubble parameter of h100=0.71. These new limits are a factor of seven better than the previous best in this frequency band. © 2012 The American Physical Society | eng |
| dc.language.iso | eng | |
| dc.publisher | College Park, MD : American Physical Society | |
| dc.relation.ispartofseries | Physical Review D 85 (2012), 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 | Gravitationswelle | ger |
| dc.subject.ddc |
530 | Physik
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ger |
| dc.title | Upper limits on a stochastic gravitational-wave background using LIGO and Virgo interferometers at 600-1000 Hz | eng |
| dc.type | Article | |
| dc.type | Text | |
| dc.relation.issn | 2470-0010 | |
| dc.relation.doi | https://doi.org/10.1103/PhysRevD.85.122001 | |
| dc.bibliographicCitation.issue | 12 | |
| dc.bibliographicCitation.volume | 85 | |
| dc.bibliographicCitation.firstPage | 122001 | |
| dc.description.version | publishedVersion | |
| tib.accessRights | frei zug�nglich |
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Fakultät für Mathematik und Physik
Frei zugängliche Publikationen aus der Fakultät für Mathematik und Physik