Phase Transitions at Preheating
High Energy Physics - Theory
2009-10-28 v3 Astrophysics
General Relativity and Quantum Cosmology
High Energy Physics - Phenomenology
Abstract
Symmetry restoration processes during the non-equilibrium stage of ``preheating'' after inflation is studied. It is shown that symmetry restoration is very efficient when the majority of created particles are concentrated at energies much smaller than the temperature in equilibrium. The strength of symmetry restoration measured in terms of the equivalent temperature can exceed by many orders of magnitude. In some models the effect can be equivalent to that if the temperature of instant reheating would be close to the Planck scale. This can have an important impact on GUT and axion models.
Cite
@article{arxiv.hep-th/9510146,
title = {Phase Transitions at Preheating},
author = {I. I. Tkachev},
journal= {arXiv preprint arXiv:hep-th/9510146},
year = {2009}
}
Comments
Some statements are corrected. Also, comments of the referee of Phys. Lett. B are taken into account; 12 pages, no figures, LaTeX