Upper limits on a stochastic gravitational-wave background using LIGO and Virgo interferometers at 600-1000 Hz
Chow, Jong; Chua, Sheon; Inta, Ra; Lam, Ping Koy; McClelland, David; Miller, John; Mow-Lowry, C; Mullavey, Adam; Nguyen, Thanh; Scott, Susan M; Shaddock, Daniel; Slagmolen, Bram; Stefszky, Michael; Wade, Andrew; Abadie, J; Abbott, B; Abbott, Robert; Anderson, S B; Araya, M; Blackburn, James Kent; Coyne, D; Etzel, T; Ivanov, A; Pedraza, M; Heefner, J; Hosken, Dave; Howell, E
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 Ω GW(f) ≥Ω...[Show more]
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|Source:||Physical Review D|
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