Stochastic background from extra-galactic double neutron stars

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dc.creatorRegimbau, T.
dc.creatorChauvineau, B.
dc.date2007-07-30
dc.date.accessioned2026-07-07T10:36:20Z
dc.date.available2026-07-07T10:36:20Z
dc.descriptionWe present Monte Carlo simulations of the extra galactic population of inspiralling double neutron stars, and estimate its contribution to the astrophysical gravitational wave background, in the frequency range of ground based interferometers, corresponding to the last thousand seconds before the last stable orbit when more than 96 percent of the signal is released. We show that sources at redshift z>0.5 contribute to a truly continuous background which may be detected by correlating third generation interferometers.
dc.description13 pages, 7 figures - proceeding of a talk given at the 11th GWDAW, to appear in CQG
dc.identifierhttps://arxiv.org/abs/0707.4327
dc.identifierhttp://arxiv.org/abs/0707.4327
dc.identifierClass.Quant.Grav.24:S627-S638,2007
dc.identifierdoi:10.1088/0264-9381/24/19/S25
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/180018
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectAstrophysics
dc.titleStochastic background from extra-galactic double neutron stars
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