A strong dissipative inflationary model
高能物理 - 唯象学
2010-11-11 v4 天体物理学
广义相对论与量子宇宙学
高能物理 - 理论
摘要
The dynamics of a single scalar field which describes a second order phase transition is considered taking into account the thermal effects in the high temperature limit. I conclude that thermal effects play a very important role during inflation and do not must to be ignored in models for the early universe. At the end of inflation thermal fluctuations are more important than quantum fluctuations, due to the fact that .
引用
@article{arxiv.hep-ph/0306067,
title = {A strong dissipative inflationary model},
author = {Mauricio Bellini},
journal= {arXiv preprint arXiv:hep-ph/0306067},
year = {2010}
}
备注
published version