Cosmic Gravitational Wave Background in String Cosmology

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dc.creatorBrustein, Ram
dc.date1998-04-29
dc.date.accessioned2026-07-07T03:32:22Z
dc.date.available2026-07-07T03:32:22Z
dc.descriptionString cosmology models predict a stochastic cosmic background of gravitational waves with a characteristic spectrum. I describe the background, present astrophysical and cosmological bounds on it, and outline how it may be possible to detect it with gravitational wave detectors.
dc.description6 pages, LaTeX, uses moriond.sty (included), 3 figures. Contribution to the proceedings of Moriond 98, Fundamental Parameters in Cosmology, Les Arcs, France (January 17-24, 1998)
dc.identifierhttps://arxiv.org/abs/gr-qc/9804078
dc.identifierhttp://arxiv.org/abs/gr-qc/9804078
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/36204
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectAstrophysics
dc.subjectHigh Energy Physics - Theory
dc.titleCosmic Gravitational Wave Background in String Cosmology
dc.typetext

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