G Giampieri and A G Polnarev 1997 Class. Quantum Grav. 14 1521 doi:10.1088/0264-9381/14/6/021
G Giampieri and A G Polnarev
Show affiliationsWe address the problem of detecting a stochastic background originated by an anisotropic population of sources, like the galactic binaries, by exploiting the amplitude modulation of the signal as the antenna changes its orientation with respect to fixed stars. This modulation, if observed, could help in discriminating the background generated by galactic binaries from the isotropic gravitational wave background generated in the early Universe.
04.80.Nn Gravitational wave detectors and experiments
Issue 6 (June 1997)
Received 16 August 1996, in final form 10 February 1997
G Giampieri and A G Polnarev 1997 Class. Quantum Grav. 14 1521
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