Quintessential inflation and non-oscillatory reheating model

dc.contributorUniversidade de São Paulo (USP)
dc.contributorUniversidade Estadual de Campinas (UNICAMP)
dc.contributorUniversidade Estadual Paulista (Unesp)
dc.date.accessioned2014-05-27T11:21:02Z
dc.date.accessioned2022-10-05T17:52:04Z
dc.date.available2014-05-27T11:21:02Z
dc.date.available2022-10-05T17:52:04Z
dc.date.created2014-05-27T11:21:02Z
dc.date.issued2004-02-01
dc.identifierNuclear Physics B - Proceedings Supplements, v. 127, p. 133-137.
dc.identifier0920-5632
dc.identifierhttp://hdl.handle.net/11449/67635
dc.identifier10.1016/S0920-5632(03)02414-9
dc.identifierWOS:000189279000023
dc.identifier2-s2.0-10744232810
dc.identifier.urihttp://repositorioslatinoamericanos.uchile.cl/handle/2250/3917265
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.
dc.languageeng
dc.relationNuclear Physics B: Proceedings Supplements
dc.rightsAcesso restrito
dc.sourceScopus
dc.titleQuintessential inflation and non-oscillatory reheating model
dc.typeArtigo


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