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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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Lenguaje: | eng |
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1999
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Acceso en línea: | http://cds.cern.ch/record/379372 |
_version_ | 1780893348679122944 |
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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 |
record_format | invenio |
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 |