Stochastic Backgrounds of Gravitational Waves from Cosmological Populations of Astrophysical Sources

Simple item page
dc.creatorSchneider, Raffaella
dc.creatorFerrari, Valeria
dc.creatorMatarrese, Sabino
dc.date1999-03-31
dc.date.accessioned2026-07-07T02:31:04Z
dc.date.available2026-07-07T02:31:04Z
dc.descriptionAstrophysical sources of gravitational radiation are likely to have been formed since the beginning of star formation. Realistic source rates of formation throughout the Universe have been estimated from an observation-based determination of the star formation rate density evolution. Both the radiation emitted during the collapse to black holes and the spin-down radiation, induced by the r-mode instability, emitted by hot, young rapidly rotating neutron stars have been considered. We have investigated the overall signal produced by the ensemble of sources exploring the parameter space and discussing its possible detectability.
dc.description9 pages, 7 figures, to appear in the proceedings of the 19th Texas Symposium on Relativistic Astrophysics and Cosmology, Paris, December 14-18, 1998
dc.identifierhttps://arxiv.org/abs/astro-ph/9903470
dc.identifierhttp://arxiv.org/abs/astro-ph/9903470
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/14033
dc.subjectAstrophysics
dc.titleStochastic Backgrounds of Gravitational Waves from Cosmological Populations of Astrophysical Sources
dc.typetext

Files

Collections

arXiv