English

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 ϕ\phi oscillates in a double-well potential and interacts with another scalar field XX, 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.

Keywords

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