期刊
ASTROPHYSICAL JOURNAL
卷 659, 期 2, 页码 918-930出版社
IOP PUBLISHING LTD
DOI: 10.1086/511329
关键词
gravitational waves
资金
- Science and Technology Facilities Council [PP/E001203/1] Funding Source: researchfish
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 90% upper limit is Omega(GW) x [H-0/72 km s(-1) Mpc(-1))](2) < 6.5 x 10(-5). This is currently the most sensitive result in the frequency range 51-150 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.
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