Dissipative Effects on Reheating after Inflation
High Energy Physics - Phenomenology
2013-03-05 v2 Cosmology and Nongalactic Astrophysics
High Energy Physics - Theory
Abstract
The inflaton must convert its energy into radiation after inflation, which, in a conventional scenario, is caused by the perturbative inflaton decay. This reheating process would be much more complicated in some cases: the decay products obtain masses from an oscillating inflaton and thermal environment, and hence the conventional reheating scenario can be modified. We study in detail processes of particle production from the inflaton, their subsequent thermalization and evolution of inflaton/plasma system by taking dissipation of the inflaton in a hot plasma into account. It is shown that the reheating temperature is significantly affected by these effects.
Keywords
Cite
@article{arxiv.1212.4985,
title = {Dissipative Effects on Reheating after Inflation},
author = {Kyohei Mukaida and Kazunori Nakayama},
journal= {arXiv preprint arXiv:1212.4985},
year = {2013}
}
Comments
22 pages, 3 figures; v2: minor changes to reflect the published version