Birth of the Universe in string cosmology

dc.creatorGasperini, M.
dc.date1997-06-13
dc.date.accessioned2026-07-07T03:31:39Z
dc.date.available2026-07-07T03:31:39Z
dc.descriptionThe decay of the string perturbative vacuum into our present cosmological state is associated to the transition from a phase of growing curvature and growing dilaton, to a phase of decreasing curvature and frozen dilaton. The possible approaches to a classical and quantum description of such a transition are introduced and briefly discussed.
dc.description17 pages, LATEX, seven figures included using EPSF, based on a talk given at the "Fourth Paris Cosmology Colloquium" (Observatoire de Paris, June 1997). To appear in the Proceedings (ed. by H. J. De Vega and N. Sanchez). 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/9706037
dc.identifierhttp://arxiv.org/abs/gr-qc/9706037
dc.identifierFourth Paris Cosmology Colloquium, eds. H.J. De Vega and N.Sanchez (World Scientific, Singapore, 1998), p. 85
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/35939
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectAstrophysics
dc.subjectHigh Energy Physics - Theory
dc.titleBirth of the Universe in string cosmology
dc.typetext

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