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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...

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Detalles Bibliográficos
Autores principales: Felder, G, Kofman, L A, Linde, Andrei D, Tkachev, Igor I
Lenguaje:eng
Publicado: 2000
Materias:
Acceso en línea:https://dx.doi.org/10.1088/1126-6708/2000/08/010
http://cds.cern.ch/record/433493
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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.
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institution Organización Europea para la Investigación Nuclear
language eng
publishDate 2000
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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