English

Inflation After Preheating

High Energy Physics - Phenomenology 2009-10-31 v1 Astrophysics General Relativity and Quantum Cosmology High Energy Physics - Theory

Abstract

Preheating after inflation may lead to nonthermal phase transitions with symmetry restoration. These phase transitions may occur even if the total energy density of fluctuations produced during reheating is relatively small as compared with the vacuum energy in the state with restored symmetry. As a result, in some inflationary models one encounters a secondary, nonthermal stage of inflation due to symmetry restoration after preheating. We review the theory of nonthermal phase transitions and make a prediction about the expansion factor during the secondary inflationary stage. We then present the results of lattice simulations which verify these predictions, and discuss possible implications of our results for the theory of formation of topological defects during nonthermal phase transitions.

Keywords

Cite

@article{arxiv.hep-ph/0004024,
  title  = {Inflation After Preheating},
  author = {Gary Felder and Lev Kofman and Andrei Linde and Igor Tkachev},
  journal= {arXiv preprint arXiv:hep-ph/0004024},
  year   = {2009}
}

Comments

22 pages, 7 figures, JHEP