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Upper limits on a stochastic gravitational-wave background using LIGO and Virgo interferometers at 600–1000 Hz

Abadie, J., Dent, Thomas Edward, Edwards, Mark, Fairhurst, Stephen ORCID: https://orcid.org/0000-0001-8480-1961, Harry, Ian William, MacDonald, Erin, MacLeod, Duncan M. ORCID: https://orcid.org/0000-0002-1395-8694, McKechan, David, Messenger, Christopher, Nuttall, Laura ORCID: https://orcid.org/0000-0002-8599-8791, Predoi, Valeriu ORCID: https://orcid.org/0000-0002-9729-6578, Sathyaprakash, Bangalore ORCID: https://orcid.org/0000-0003-3845-7586, Schutz, Bernard Frederick ORCID: https://orcid.org/0000-0001-9487-6983, Sutton, Patrick J. ORCID: https://orcid.org/0000-0003-1614-3922, Veitch, John, LIGO Scientific Collaboration and Virgo Collaboration 2012. Upper limits on a stochastic gravitational-wave background using LIGO and Virgo interferometers at 600–1000 Hz. Physical Review D Particles and Fields 85 (12) , 122001. 10.1103/PhysRevD.85.122001

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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.

Item Type: Article
Date Type: Publication
Status: Published
Schools: Physics and Astronomy
Subjects: Q Science > QB Astronomy
Additional Information: Please go to publisher's page for full list of contributors to this paper.
Publisher: American Physical Society
ISSN: 0556-2821
Last Modified: 10 Mar 2024 17:34
URI: https://orca.cardiff.ac.uk/id/eprint/47553

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