Upper Limits on the Stochastic Background of Gravitational Waves
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 0 < 8.4 × 10 -4 in the 69-156 Hz...[Show more]
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|Source:||Physical Review Letters|
|01_McClelland_Upper_Limits_on_the_Stochastic_2005.pdf||719.91 kB||Adobe PDF||Request a copy|
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