J Alberto Lobo and Álvaro Montero 2002 Class. Quantum Grav. 19 6405 doi:10.1088/0264-9381/19/24/309
J Alberto Lobo and Álvaro Montero
Show affiliationsThe analysis of how a stochastic background of gravitational radiation interacts with a spherical detector is given in detail, which leads to explicit expressions for the system response functions, as well as for the cross-correlation matrix of different readout channels. It is shown that distinctive features of GW-induced random detector excitations, relative to locally generated noise, are, in practice, insufficient for separating the signal from the noise by means of a single sphere.
Issue 24 (21 December 2002)
Received 4 June 2002, in final form 16 October 2002
Published 28 November 2002
J Alberto Lobo and Álvaro Montero 2002 Class. Quantum Grav. 19 6405
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