Loading [MathJax]/extensions/tex2jax.js

Searching for a stochastic background of gravitational waves with the laser interferometer gravitational-wave observatory

Publikation: Beitrag in Fachzeitschrift › Artikel › Forschung › Peer-Review

Autorschaft

  • The LIGO Scientific Collaboration

Organisationseinheiten

Externe Organisationen

  • Ochanomizu University

Details

Originalspracheundefiniert/unbekannt
Seiten (von - bis)918-930
Seitenumfang13
FachzeitschriftAstrophysical Journal
Jahrgang659
Ausgabenummer2
PublikationsstatusVeröffentlicht - 2007

Abstract

The Laser Interferometer Gravitational-Wave Observatory (LIGO) has performed the fourth science run, S4, with significantly improved interferometer sensitivities with respect to previous runs. Using data acquired during this science run, we place a limit on the amplitude of a stochastic background of gravitational waves. For a frequency independent spectrum, the new Bayesian 90150 Hz, with a factor of 13 improvement over the previous LIGO result. We discuss the complementarity of the new result with other constraints on a stochastic background of gravitational waves, and we investigate implications of the new result for different models of this background.

Zitieren

Searching for a stochastic background of gravitational waves with the laser interferometer gravitational-wave observatory. / The LIGO Scientific Collaboration.
in: Astrophysical Journal, Jahrgang 659, Nr. 2, 2007, S. 918-930.

Publikation: Beitrag in Fachzeitschrift › Artikel › Forschung › Peer-Review

Download
@article{cc7e1b4b62534e1682fcb550ef4b83c3,
title = "Searching for a stochastic background of gravitational waves with the laser interferometer gravitational-wave observatory",
abstract = "The Laser Interferometer Gravitational-Wave Observatory (LIGO) has performed the fourth science run, S4, with significantly improved interferometer sensitivities with respect to previous runs. Using data acquired during this science run, we place a limit on the amplitude of a stochastic background of gravitational waves. For a frequency independent spectrum, the new Bayesian 90150 Hz, with a factor of 13 improvement over the previous LIGO result. We discuss the complementarity of the new result with other constraints on a stochastic background of gravitational waves, and we investigate implications of the new result for different models of this background.",
author = "{The LIGO Scientific Collaboration} and B. Abbott and R. Abbott and R. Adhikari and J. Agresti and P. Ajith and B. Allen and R. Amin and Anderson, {S. B.} and Anderson, {W. G.} and M. Araya and H. Armandula and M. Ashley and S Aston and C. Aulbert and Stanislav Babak and S. Ballmer and Barish, {B. C.} and C. Barker and D. Barker and B. Barr and P. Barriga and Barton, {M. A.} and K. Bayer and K. Belczynski and J. Betzwieser and P. Beyersdorf and B. Bhawal and Bilenko, {I. A.} and G. Billingsley and E. Black and K. Blackburn and L. Blackburn and D. Blair and B. Bland and L. Bogue and S. Bose and Brown, {D. A.} and Y. Chen and K. Danzmann and A. Dietz and T. Fricke and M. Heurs and M. Hewitson and F. Kawazoe and A. Khan and H. L{\"u}ck and H. Vahlbruch and B. Willke and W. Wu and L. Zhang",
year = "2007",
doi = "10.1086/511329",
language = "Undefined/Unknown",
volume = "659",
pages = "918--930",
journal = "Astrophysical Journal",
issn = "1538-4357",
publisher = "IOP Publishing Ltd.",
number = "2",

}

Download

TY - JOUR

T1 - Searching for a stochastic background of gravitational waves with the laser interferometer gravitational-wave observatory

AU - The LIGO Scientific Collaboration

AU - Abbott, B.

AU - Abbott, R.

AU - Adhikari, R.

AU - Agresti, J.

AU - Ajith, P.

AU - Allen, B.

AU - Amin, R.

AU - Anderson, S. B.

AU - Anderson, W. G.

AU - Araya, M.

AU - Armandula, H.

AU - Ashley, M.

AU - Aston, S

AU - Aulbert, C.

AU - Babak, Stanislav

AU - Ballmer, S.

AU - Barish, B. C.

AU - Barker, C.

AU - Barker, D.

AU - Barr, B.

AU - Barriga, P.

AU - Barton, M. A.

AU - Bayer, K.

AU - Belczynski, K.

AU - Betzwieser, J.

AU - Beyersdorf, P.

AU - Bhawal, B.

AU - Bilenko, I. A.

AU - Billingsley, G.

AU - Black, E.

AU - Blackburn, K.

AU - Blackburn, L.

AU - Blair, D.

AU - Bland, B.

AU - Bogue, L.

AU - Bose, S.

AU - Brown, D. A.

AU - Chen, Y.

AU - Danzmann, K.

AU - Dietz, A.

AU - Fricke, T.

AU - Heurs, M.

AU - Hewitson, M.

AU - Kawazoe, F.

AU - Khan, A.

AU - Lück, H.

AU - Vahlbruch, H.

AU - Willke, B.

AU - Wu, W.

AU - Zhang, L.

PY - 2007

Y1 - 2007

N2 - The Laser Interferometer Gravitational-Wave Observatory (LIGO) has performed the fourth science run, S4, with significantly improved interferometer sensitivities with respect to previous runs. Using data acquired during this science run, we place a limit on the amplitude of a stochastic background of gravitational waves. For a frequency independent spectrum, the new Bayesian 90150 Hz, with a factor of 13 improvement over the previous LIGO result. We discuss the complementarity of the new result with other constraints on a stochastic background of gravitational waves, and we investigate implications of the new result for different models of this background.

AB - The Laser Interferometer Gravitational-Wave Observatory (LIGO) has performed the fourth science run, S4, with significantly improved interferometer sensitivities with respect to previous runs. Using data acquired during this science run, we place a limit on the amplitude of a stochastic background of gravitational waves. For a frequency independent spectrum, the new Bayesian 90150 Hz, with a factor of 13 improvement over the previous LIGO result. We discuss the complementarity of the new result with other constraints on a stochastic background of gravitational waves, and we investigate implications of the new result for different models of this background.

U2 - 10.1086/511329

DO - 10.1086/511329

M3 - Article

VL - 659

SP - 918

EP - 930

JO - Astrophysical Journal

JF - Astrophysical Journal

SN - 1538-4357

IS - 2

ER -

Von denselben Autoren