Testing string cosmology with gravity wave detectors

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dc.creatorGasperini, M.
dc.date1997-07-15
dc.date.accessioned2026-07-07T03:31:42Z
dc.date.available2026-07-07T03:31:42Z
dc.descriptionThe general properties of the gravity wave backgrounds of cosmological origin are reviewed and briefly discussed, with emphasis on the relic background expected from an early pre-big bang phase typical of string cosmology models.
dc.description13 pages, LATEX, three figures included using EPSFIG. Talk given at the "Second Edoardo Amaldi Conference on Gravitational Wawes" (CERN, 1-4 July 1997). To be published in the Proceedings (World Scientific, Singapore), eds E. Coccia et al. An updated collection of papers on the pre-big bang scenario is available at http://www.to.infn.it/teorici/gasperini
dc.identifierhttps://arxiv.org/abs/gr-qc/9707034
dc.identifierhttp://arxiv.org/abs/gr-qc/9707034
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/35955
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectAstrophysics
dc.subjectHigh Energy Physics - Phenomenology
dc.subjectHigh Energy Physics - Theory
dc.titleTesting string cosmology with gravity wave detectors
dc.typetext

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