Abadie, J., Dent, Thomas Edward, Edwards, Mark, Fairhurst, Stephen ![]() ![]() ![]() ![]() ![]() ![]() ![]() |
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 |
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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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