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Inflating, Warming Up and Probing the Pre-Bangian Universe

Classical and quantum gravitational instabilities, can, respectively, inflate and warm up a primordial Universe satisfying a superstring-motivated principle of "Asymptotic Past Triviality". A physically viable big bang is thus generated without invoking either large fine-tunings or a long...

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Autor principal: Veneziano, Gabriele
Lenguaje:eng
Publicado: 1999
Materias:
Acceso en línea:http://cds.cern.ch/record/379372
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author Veneziano, Gabriele
author_facet Veneziano, Gabriele
author_sort Veneziano, Gabriele
collection CERN
description Classical and quantum gravitational instabilities, can, respectively, inflate and warm up a primordial Universe satisfying a superstring-motivated principle of "Asymptotic Past Triviality". A physically viable big bang is thus generated without invoking either large fine-tunings or a long period of post-big bang inflation. Properties of the pre-bangian Universe can be probed through its observable relics, which include: i) a (possibly observable) stochastic gravitational-wave background; ii) a (possible) new mechanism for seeding the galactic magnetic fields; iii) a (possible) new source of large-scale structure and CMB anisotropy.
id cern-379372
institution Organización Europea para la Investigación Nuclear
language eng
publishDate 1999
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spelling cern-3793722022-03-31T02:28:52Zhttp://cds.cern.ch/record/379372engVeneziano, GabrieleInflating, Warming Up and Probing the Pre-Bangian UniverseParticle Physics - TheoryClassical and quantum gravitational instabilities, can, respectively, inflate and warm up a primordial Universe satisfying a superstring-motivated principle of "Asymptotic Past Triviality". A physically viable big bang is thus generated without invoking either large fine-tunings or a long period of post-big bang inflation. Properties of the pre-bangian Universe can be probed through its observable relics, which include: i) a (possibly observable) stochastic gravitational-wave background; ii) a (possible) new mechanism for seeding the galactic magnetic fields; iii) a (possible) new source of large-scale structure and CMB anisotropy.Classical and quantum gravitational instabilities, can, respectively, inflate and warm up a primordial Universe satisfying a superstring-motivated principle of "Asymptotic Past Triviality". A physically viable big bang is thus generated without invoking either large fine-tunings or a long period of post-big bang inflation. Properties of the pre-bangian Universe can be probed through its observable relics, which include: i) a (possibly observable) stochastic gravitational-wave background; ii) a (possible) new mechanism for seeding the galactic magnetic fields; iii) a (possible) new source of large-scale structure and CMB anisotropy.hep-th/9902097CERN-TH-99-22CERN-TH-99-022oai:cds.cern.ch:3793721999-02-15
spellingShingle Particle Physics - Theory
Veneziano, Gabriele
Inflating, Warming Up and Probing the Pre-Bangian Universe
title Inflating, Warming Up and Probing the Pre-Bangian Universe
title_full Inflating, Warming Up and Probing the Pre-Bangian Universe
title_fullStr Inflating, Warming Up and Probing the Pre-Bangian Universe
title_full_unstemmed Inflating, Warming Up and Probing the Pre-Bangian Universe
title_short Inflating, Warming Up and Probing the Pre-Bangian Universe
title_sort inflating, warming up and probing the pre-bangian universe
topic Particle Physics - Theory
url http://cds.cern.ch/record/379372
work_keys_str_mv AT venezianogabriele inflatingwarmingupandprobingtheprebangianuniverse