Curvaton reheating in tachyonic inflationary models

dc.contributor.author	Campuzano, C.
dc.contributor.author	Del Campo, S.
dc.contributor.author	Herrera, R.
dc.date.accessioned	2021-07-06T18:16:33Z
dc.date.available	2021-07-06T18:16:33Z
dc.date.issued	2006-02
dc.description	Indexación: Scopus.	es
dc.description.abstract	The curvaton reheating in a tachyonic inflationary universe model with an exponential potential is studied. We have found that the energy density in the kinetic epoch, has a complicated dependencies of the scale factor. For different scenarios, the temperature of reheating is computed. These temperature result to be analogous to those obtained in the standard case of the curvaton scenario.	es
dc.description.uri	https://www.sciencedirect.com/science/article/pii/S0370269305017314?via%3Dihub
dc.identifier.citation	Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics, Volume 633, Issue 2-3, Pages 149 - 154, 9 February 2006	es
dc.identifier.doi	DOI: 10.1016/j.physletb.2005.11.058
dc.identifier.issn	0370-2693
dc.identifier.uri	http://repositorio.unab.cl/xmlui/handle/ria/19276
dc.language.iso	en	es
dc.publisher	Elsevier [Commercial Publisher] North-Holland [Associate Organisation]	es
dc.subject	Inflation	es
dc.subject	Supergravity	es
dc.subject	Bispectrum	es
dc.title	Curvaton reheating in tachyonic inflationary models	es
dc.type	Artículo	es

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