Inhomogeneous Pre-Big Bang String Cosmology

An inhomogeneous version of Pre--Big Bang cosmology emerges, within string theory, from quite generic initial conditions, provided they lie deeply inside the weak-coupling, low-curvature regime. Large-scale homogeneity, flatness, and isotropy appear naturally as late-time outcomes of such an evoluti...

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Detalles Bibliográficos
Autor principal: Veneziano, G.
Lenguaje:eng
Publicado: 1997
Materias:
Particle Physics - Theory
Acceso en línea:https://dx.doi.org/10.1016/S0370-2693(97)00688-6
http://cds.cern.ch/record/322851
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author Veneziano, G.
author_facet Veneziano, G.
author_sort Veneziano, G.
collection CERN
description An inhomogeneous version of Pre--Big Bang cosmology emerges, within string theory, from quite generic initial conditions, provided they lie deeply inside the weak-coupling, low-curvature regime. Large-scale homogeneity, flatness, and isotropy appear naturally as late-time outcomes of such an evolution.
id cern-322851
institution Organización Europea para la Investigación Nuclear
language eng
publishDate 1997
record_format invenio
spelling cern-3228512023-03-14T17:10:02Zdoi:10.1016/S0370-2693(97)00688-6http://cds.cern.ch/record/322851engVeneziano, G.Inhomogeneous Pre-Big Bang String CosmologyParticle Physics - TheoryAn inhomogeneous version of Pre--Big Bang cosmology emerges, within string theory, from quite generic initial conditions, provided they lie deeply inside the weak-coupling, low-curvature regime. Large-scale homogeneity, flatness, and isotropy appear naturally as late-time outcomes of such an evolution.An inhomogeneous version of Pre--Big Bang cosmology emerges, within string theory, from quite generic initial conditions, provided they lie deeply inside the weak-coupling, low-curvature regime. Large-scale homogeneity, flatness, and isotropy appear naturally as late-time outcomes of such an evolution.An inhomogeneous version of pre-Big Bang cosmology emerges, within string theory, from quite generic initial conditions, provided they lie deeply inside the weak-coupling, low-curvature regime. Large-scale homogeneity, flatness, and isotropy appear naturally as late-time outcomes of such an evolution.hep-th/9703150CERN-TH-97-042CERN-TH-97-42CERN-TH-97-042oai:cds.cern.ch:3228511997-03-24
spellingShingle Particle Physics - Theory
Veneziano, G.
Inhomogeneous Pre-Big Bang String Cosmology
title Inhomogeneous Pre-Big Bang String Cosmology
title_full Inhomogeneous Pre-Big Bang String Cosmology
title_fullStr Inhomogeneous Pre-Big Bang String Cosmology
title_full_unstemmed Inhomogeneous Pre-Big Bang String Cosmology
title_short Inhomogeneous Pre-Big Bang String Cosmology
title_sort inhomogeneous pre-big bang string cosmology
topic Particle Physics - Theory
url https://dx.doi.org/10.1016/S0370-2693(97)00688-6
http://cds.cern.ch/record/322851
work_keys_str_mv AT venezianog inhomogeneousprebigbangstringcosmology

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