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dc.contributor.authorCampos, A. H.
dc.contributor.authorReis, H. C.
dc.contributor.authorRosenfeld, Rogério [UNESP]
dc.date.accessioned2014-05-27T11:21:02Z
dc.date.available2014-05-27T11:21:02Z
dc.date.issued2004-02-01
dc.identifierhttp://dx.doi.org/10.1016/S0920-5632(03)02414-9
dc.identifier.citationNuclear Physics B - Proceedings Supplements, v. 127, p. 133-137.
dc.identifier.issn0920-5632
dc.identifier.urihttp://hdl.handle.net/11449/67635
dc.description.abstractA numerical study of the non-oscillatory reheating mechanism in a quintessential inflation context shows that high reheating temperature can be achieved compared with the usual reheating mechanism in which particles are produced gravitationally. We find that even for a very small coupling between the inflaton field and a massless scalar field, the non-oscillatory reheating production of particles dominates over the gravitational production mechanism. © 2004 Published by Elsevier B.V.en
dc.format.extent133-137
dc.language.isoeng
dc.relation.ispartofNuclear Physics B: Proceedings Supplements
dc.sourceScopus
dc.titleQuintessential inflation and non-oscillatory reheating modelen
dc.typeArtigo
dcterms.licensehttp://www.elsevier.com/about/open-access/open-access-policies/article-posting-policy
dc.contributor.institutionUniversidade de São Paulo (USP)
dc.contributor.institutionUniversidade Estadual de Campinas (UNICAMP)
dc.contributor.institutionUniversidade Estadual Paulista (UNESP)
dc.description.affiliationInstituto de Física - USP Departamento de Fisica Nuclear, CP 66318, São Paulo, SP
dc.description.affiliationInst. Fisica Gleb Wataghin-UNICAMP Depto. de Raios Cosmicos Cronologia, CP 6165, Campinas, SP
dc.description.affiliationInstituto de Fisica Teorica-UNESP, Rua Pamplona 145, 01405-900- São, SP
dc.description.affiliationUnespInstituto de Fisica Teorica-UNESP, Rua Pamplona 145, 01405-900- São, SP
dc.identifier.doi10.1016/S0920-5632(03)02414-9
dc.identifier.wosWOS:000189279000023
dc.rights.accessRightsAcesso restrito
dc.identifier.scopus2-s2.0-10744232810
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