First-order nonthermal phase transition after preheating
High Energy Physics - Phenomenology
2009-09-29 v1 Astrophysics
General Relativity and Quantum Cosmology
High Energy Physics - Theory
Abstract
During preheating after inflation, parametric resonance rapidly generates very large fluctuations of scalar fields. In models where the inflaton field oscillates in a double-well potential and interacts with another scalar field , fluctuations of X can keep the \phi to -\phi symmetry temporarily restored. If the coupling of \phi to X is much stronger than the inflaton self-coupling, the subsequent symmetry breaking is a first-order phase transition. We demonstrate the existence of this nonthermal phase transition with lattice simulations of the full nonlinear dynamics of the interacting fields. In particular, we observe nucleation of an expanding bubble.
Cite
@article{arxiv.hep-ph/9804425,
title = {First-order nonthermal phase transition after preheating},
author = {S. Khlebnikov and L. Kofman and A. Linde and I. Tkachev},
journal= {arXiv preprint arXiv:hep-ph/9804425},
year = {2009}
}
Comments
RevTeX, 4 pages