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Inflation After Preheating
Preheating after inflation may lead to nonthermal phase transitions with symmetry restoration. These phase transitions may occur even if the total energy density of fluctuations produced during reheating is relatively small as compared with the vacuum energy in the state with restored symmetry. As a...
Autores principales: | , , , |
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Lenguaje: | eng |
Publicado: |
2000
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Materias: | |
Acceso en línea: | https://dx.doi.org/10.1088/1126-6708/2000/08/010 http://cds.cern.ch/record/433493 |
_version_ | 1780895333303189504 |
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author | Felder, G Kofman, L A Linde, Andrei D Tkachev, Igor I |
author_facet | Felder, G Kofman, L A Linde, Andrei D Tkachev, Igor I |
author_sort | Felder, G |
collection | CERN |
description | Preheating after inflation may lead to nonthermal phase transitions with symmetry restoration. These phase transitions may occur even if the total energy density of fluctuations produced during reheating is relatively small as compared with the vacuum energy in the state with restored symmetry. As a result, in some inflationary models one encounters a secondary, nonthermal stage of inflation due to symmetry restoration after preheating. We review the theory of nonthermal phase transitions and make a prediction about the expansion factor during the secondary inflationary stage. We then present the results of lattice simulations which verify these predictions, and discuss possible implications of our results for the theory of formation of topological defects during nonthermal phase transitions. |
id | cern-433493 |
institution | Organización Europea para la Investigación Nuclear |
language | eng |
publishDate | 2000 |
record_format | invenio |
spelling | cern-4334932019-09-30T06:29:59Zdoi:10.1088/1126-6708/2000/08/010http://cds.cern.ch/record/433493engFelder, GKofman, L ALinde, Andrei DTkachev, Igor IInflation After PreheatingParticle Physics - PhenomenologyPreheating after inflation may lead to nonthermal phase transitions with symmetry restoration. These phase transitions may occur even if the total energy density of fluctuations produced during reheating is relatively small as compared with the vacuum energy in the state with restored symmetry. As a result, in some inflationary models one encounters a secondary, nonthermal stage of inflation due to symmetry restoration after preheating. We review the theory of nonthermal phase transitions and make a prediction about the expansion factor during the secondary inflationary stage. We then present the results of lattice simulations which verify these predictions, and discuss possible implications of our results for the theory of formation of topological defects during nonthermal phase transitions.hep-ph/0004024CERN-TH-2000-069CITA-2000-06oai:cds.cern.ch:4334932000-04-04 |
spellingShingle | Particle Physics - Phenomenology Felder, G Kofman, L A Linde, Andrei D Tkachev, Igor I Inflation After Preheating |
title | Inflation After Preheating |
title_full | Inflation After Preheating |
title_fullStr | Inflation After Preheating |
title_full_unstemmed | Inflation After Preheating |
title_short | Inflation After Preheating |
title_sort | inflation after preheating |
topic | Particle Physics - Phenomenology |
url | https://dx.doi.org/10.1088/1126-6708/2000/08/010 http://cds.cern.ch/record/433493 |
work_keys_str_mv | AT felderg inflationafterpreheating AT kofmanla inflationafterpreheating AT lindeandreid inflationafterpreheating AT tkachevigori inflationafterpreheating |