Preheating in quintessential inflation
| Autor(a) principal: | |
|---|---|
| Data de Publicação: | 2003 |
| Outros Autores: | , |
| Tipo de documento: | Artigo |
| Idioma: | eng |
| Título da fonte: | Repositório Institucional da UNESP |
| Texto Completo: | http://dx.doi.org/10.1016/j.physletb.2003.09.064 http://hdl.handle.net/11449/67476 |
Resumo: | We perform a numerical study of the preheating mechanism of particle production in models of quintessential inflation and compare it with the usual gravitational production mechanism. We find that even for a very small coupling between the inflaton field and a massless scalar field, g ≳ 10 -6, preheating dominates over gravitational particle production. Reheating temperatures in the range 10 4 ≲ T rh ≲ 10 15 GeV can be easily obtained. © 2003 Published by Elsevier B.V. |
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Preheating in quintessential inflationcosmoselementary particleevolutiongravityheatingmasstemperatureWe perform a numerical study of the preheating mechanism of particle production in models of quintessential inflation and compare it with the usual gravitational production mechanism. We find that even for a very small coupling between the inflaton field and a massless scalar field, g ≳ 10 -6, preheating dominates over gravitational particle production. Reheating temperatures in the range 10 4 ≲ T rh ≲ 10 15 GeV can be easily obtained. © 2003 Published by Elsevier B.V.Instituto de Física USP Departamento de Fisica Nuclear, CP 66318, São Paulo, SPInstituto de Fisica Gleb Wataghin UNICAMP Depto. de Raios Cosmic. e Cronologia, CP 6165, Campinas, SPInstituto de Fisica Teorica UNESP, Rua Pamplona 145, 01405-900 São Paulo, SPInstituto de Fisica Teorica UNESP, Rua Pamplona 145, 01405-900 São Paulo, SPUniversidade de São Paulo (USP)Universidade Estadual de Campinas (UNICAMP)Universidade Estadual Paulista (Unesp)Campos, A. H.Reis, H. C.Rosenfeld, Rogério [UNESP]2014-05-27T11:20:56Z2014-05-27T11:20:56Z2003-11-27info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/article151-156application/pdfhttp://dx.doi.org/10.1016/j.physletb.2003.09.064Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics, v. 575, n. 3-4, p. 151-156, 2003.0370-2693http://hdl.handle.net/11449/6747610.1016/j.physletb.2003.09.0642-s2.0-171444482262-s2.0-17144448226.pdfScopusreponame:Repositório Institucional da UNESPinstname:Universidade Estadual Paulista (UNESP)instacron:UNESPengPhysics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics4.2542,336info:eu-repo/semantics/openAccess2024-01-22T06:20:51Zoai:repositorio.unesp.br:11449/67476Repositório InstitucionalPUBhttp://repositorio.unesp.br/oai/requestopendoar:29462024-08-05T23:38:11.421571Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP)false |
| dc.title.none.fl_str_mv |
Preheating in quintessential inflation |
| title |
Preheating in quintessential inflation |
| spellingShingle |
Preheating in quintessential inflation Campos, A. H. cosmos elementary particle evolution gravity heating mass temperature |
| title_short |
Preheating in quintessential inflation |
| title_full |
Preheating in quintessential inflation |
| title_fullStr |
Preheating in quintessential inflation |
| title_full_unstemmed |
Preheating in quintessential inflation |
| title_sort |
Preheating in quintessential inflation |
| author |
Campos, A. H. |
| author_facet |
Campos, A. H. Reis, H. C. Rosenfeld, Rogério [UNESP] |
| author_role |
author |
| author2 |
Reis, H. C. Rosenfeld, Rogério [UNESP] |
| author2_role |
author author |
| dc.contributor.none.fl_str_mv |
Universidade de São Paulo (USP) Universidade Estadual de Campinas (UNICAMP) Universidade Estadual Paulista (Unesp) |
| dc.contributor.author.fl_str_mv |
Campos, A. H. Reis, H. C. Rosenfeld, Rogério [UNESP] |
| dc.subject.por.fl_str_mv |
cosmos elementary particle evolution gravity heating mass temperature |
| topic |
cosmos elementary particle evolution gravity heating mass temperature |
| description |
We perform a numerical study of the preheating mechanism of particle production in models of quintessential inflation and compare it with the usual gravitational production mechanism. We find that even for a very small coupling between the inflaton field and a massless scalar field, g ≳ 10 -6, preheating dominates over gravitational particle production. Reheating temperatures in the range 10 4 ≲ T rh ≲ 10 15 GeV can be easily obtained. © 2003 Published by Elsevier B.V. |
| publishDate |
2003 |
| dc.date.none.fl_str_mv |
2003-11-27 2014-05-27T11:20:56Z 2014-05-27T11:20:56Z |
| dc.type.status.fl_str_mv |
info:eu-repo/semantics/publishedVersion |
| dc.type.driver.fl_str_mv |
info:eu-repo/semantics/article |
| format |
article |
| status_str |
publishedVersion |
| dc.identifier.uri.fl_str_mv |
http://dx.doi.org/10.1016/j.physletb.2003.09.064 Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics, v. 575, n. 3-4, p. 151-156, 2003. 0370-2693 http://hdl.handle.net/11449/67476 10.1016/j.physletb.2003.09.064 2-s2.0-17144448226 2-s2.0-17144448226.pdf |
| url |
http://dx.doi.org/10.1016/j.physletb.2003.09.064 http://hdl.handle.net/11449/67476 |
| identifier_str_mv |
Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics, v. 575, n. 3-4, p. 151-156, 2003. 0370-2693 10.1016/j.physletb.2003.09.064 2-s2.0-17144448226 2-s2.0-17144448226.pdf |
| dc.language.iso.fl_str_mv |
eng |
| language |
eng |
| dc.relation.none.fl_str_mv |
Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics 4.254 2,336 |
| dc.rights.driver.fl_str_mv |
info:eu-repo/semantics/openAccess |
| eu_rights_str_mv |
openAccess |
| dc.format.none.fl_str_mv |
151-156 application/pdf |
| dc.source.none.fl_str_mv |
Scopus reponame:Repositório Institucional da UNESP instname:Universidade Estadual Paulista (UNESP) instacron:UNESP |
| instname_str |
Universidade Estadual Paulista (UNESP) |
| instacron_str |
UNESP |
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UNESP |
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Repositório Institucional da UNESP |
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Repositório Institucional da UNESP |
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Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP) |
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1808129538883846144 |