Quintessential inflation and non-oscillatory reheating model
Contribuinte(s) |
Universidade Estadual Paulista (UNESP) |
---|---|
Data(s) |
27/05/2014
27/05/2014
01/02/2004
|
Resumo |
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. |
Formato |
133-137 |
Identificador |
http://dx.doi.org/10.1016/S0920-5632(03)02414-9 Nuclear Physics B - Proceedings Supplements, v. 127, p. 133-137. 0920-5632 http://hdl.handle.net/11449/67635 10.1016/S0920-5632(03)02414-9 WOS:000189279000023 2-s2.0-10744232810 |
Idioma(s) |
eng |
Relação |
Nuclear Physics B: Proceedings Supplements |
Direitos |
closedAccess |
Tipo |
info:eu-repo/semantics/article |