Please use this identifier to cite or link to this item: http://hdl.handle.net/2440/48818
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Type: Journal article
Title: Upper limits on a stochastic background of gravitational waves
Author: Abbott, B.
Abbott, R.
Adhikari, R.
Agresti, J.
Allen, B.
Allen, G.
Amin, R.
Anderson, S.
Anderson, W.
Araya, M.
Armandula, H.
Ashley, M.
Aulbert, C.
Babak, S.
Balasubramanian, R.
Ballmer, S.
Barish, B.
Barker, C.
Barker, D.
Barton, M.
et al.
Citation: Physical Review Letters, 2005; 95(22):221101-1-221101-6
Publisher: American Physical Soc
Issue Date: 2005
ISSN: 0031-9007
1079-7114
Statement of
Responsibility: 
B. Abbott... D. J. Ottaway... et al.(LIGO Scientific Collaboration)
Abstract: The Laser Interferometer Gravitational-Wave Observatory has performed a third science run with much improved sensitivities of all three interferometers. We present an analysis of approximately 200 hours of data acquired during this run, used to search for a stochastic background of gravitational radiation. We place upper bounds on the energy density stored as gravitational radiation for three different spectral power laws. For the flat spectrum, our limit of Ω0<8.4×10-4 in the 69–156 Hz band is ∼105 times lower than the previous result in this frequency range.
Keywords: LIGO Scientific Collaboration
Rights: ©2005 American Physical Society
RMID: 0020083081
DOI: 10.1103/PhysRevLett.95.221101
Appears in Collections:Physics publications

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