Please use this identifier to cite or link to this item:
http://acervodigital.unesp.br/handle/11449/67635
- Title:
- Quintessential inflation and non-oscillatory reheating model
- Universidade de São Paulo (USP)
- Universidade Estadual de Campinas (UNICAMP)
- Universidade Estadual Paulista (UNESP)
- 0920-5632
- A 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.
- 1-Feb-2004
- Nuclear Physics B - Proceedings Supplements, v. 127, p. 133-137.
- 133-137
- http://dx.doi.org/10.1016/S0920-5632(03)02414-9
- Acesso restrito
- outro
- http://repositorio.unesp.br/handle/11449/67635
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