Sensitivity of a VIRGO pair to relic gravitational wave backgrounds

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Published under licence by IOP Publishing Ltd
, , Citation D Babusci and M Giovannini 2000 Class. Quantum Grav. 17 2621 DOI 10.1088/0264-9381/17/14/302

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1 INFN-Laboratori Nazionali di Frascati, 1-00044 Frascati, Italy

2 Institute for Theoretical Physics, Lausanne University, BSP-Dorigny, CH-1015, Switzerland

Dates

  1. Received 21 December 1999

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0264-9381/17/14/2621

Abstract

The sensitivity of a pair of VIRGO interferometers to gravitational wave (GW) backgrounds of cosmological origin is analysed for the cases of maximal and minimal overlap of the two detectors. The improvements in the detectability prospects of scale-invariant and non-scale-invariant logarithmic energy spectra of relic GW are discussed.

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