Publicação: Preheating in quintessential inflation
dc.contributor.author | Campos, A. H. | |
dc.contributor.author | Reis, H. C. | |
dc.contributor.author | Rosenfeld, Rogério [UNESP] | |
dc.contributor.institution | Universidade de São Paulo (USP) | |
dc.contributor.institution | Universidade Estadual de Campinas (UNICAMP) | |
dc.contributor.institution | Universidade Estadual Paulista (Unesp) | |
dc.date.accessioned | 2014-05-27T11:20:56Z | |
dc.date.available | 2014-05-27T11:20:56Z | |
dc.date.issued | 2003-11-27 | |
dc.description.abstract | 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. | en |
dc.description.affiliation | Instituto de Física USP Departamento de Fisica Nuclear, CP 66318, São Paulo, SP | |
dc.description.affiliation | Instituto de Fisica Gleb Wataghin UNICAMP Depto. de Raios Cosmic. e Cronologia, CP 6165, Campinas, SP | |
dc.description.affiliation | Instituto de Fisica Teorica UNESP, Rua Pamplona 145, 01405-900 São Paulo, SP | |
dc.description.affiliationUnesp | Instituto de Fisica Teorica UNESP, Rua Pamplona 145, 01405-900 São Paulo, SP | |
dc.format.extent | 151-156 | |
dc.identifier | http://dx.doi.org/10.1016/j.physletb.2003.09.064 | |
dc.identifier.citation | Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics, v. 575, n. 3-4, p. 151-156, 2003. | |
dc.identifier.doi | 10.1016/j.physletb.2003.09.064 | |
dc.identifier.file | 2-s2.0-17144448226.pdf | |
dc.identifier.issn | 0370-2693 | |
dc.identifier.scopus | 2-s2.0-17144448226 | |
dc.identifier.uri | http://hdl.handle.net/11449/67476 | |
dc.language.iso | eng | |
dc.relation.ispartof | Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics | |
dc.relation.ispartofjcr | 4.254 | |
dc.relation.ispartofsjr | 2,336 | |
dc.rights.accessRights | Acesso aberto | |
dc.source | Scopus | |
dc.subject | cosmos | |
dc.subject | elementary particle | |
dc.subject | evolution | |
dc.subject | gravity | |
dc.subject | heating | |
dc.subject | mass | |
dc.subject | temperature | |
dc.title | Preheating in quintessential inflation | en |
dc.type | Artigo | |
dcterms.license | http://www.elsevier.com/about/open-access/open-access-policies/article-posting-policy | |
dspace.entity.type | Publication | |
unesp.campus | Universidade Estadual Paulista (UNESP), Instituto de Física Teórica (IFT), São Paulo | pt |
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