Prospects for Stochastic Background Searches Using Virgo and LSC Interferometers

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dc.creatorCella, Giancarlo
dc.creatorColacino, Carlo Nicola
dc.creatorCuoco, Elena
dc.creatorDi Virgilio, Angela
dc.creatorRegimbau, Tania
dc.creatorRobinson, Emma L
dc.creatorWhelan, John T
dc.date2007-04-23
dc.date2007-07-09
dc.date.accessioned2026-07-07T10:35:41Z
dc.date.available2026-07-07T10:35:41Z
dc.descriptionWe consider the question of cross-correlation measurements using Virgo and the LSC Interferometers (LIGO Livingston, LIGO Hanford, and GEO600) to search for a stochastic gravitational-wave background. We find that inclusion of Virgo into the network will substantially improve the sensitivity to correlations above 200 Hz if all detectors are operating at their design sensitivity. This is illustrated using a simulated isotropic stochastic background signal, generated with an astrophysically-motivated spectrum, injected into 24 hours of simulated noise for the LIGO and Virgo interferometers.
dc.description11 pages, uses IOP style files, submitted to CQG for GWDAW11 proceedings; revised in response to referee comments
dc.identifierhttps://arxiv.org/abs/0704.2983
dc.identifierhttp://arxiv.org/abs/0704.2983
dc.identifierClass.Quant.Grav.24:S639-S648,2007
dc.identifierdoi:10.1088/0264-9381/24/19/S26
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/179811
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleProspects for Stochastic Background Searches Using Virgo and LSC Interferometers
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