English

Structure of Resonance in Preheating after Inflation

High Energy Physics - Phenomenology 2009-09-29 v1 Astrophysics General Relativity and Quantum Cosmology High Energy Physics - Theory

Abstract

We consider preheating in the theory 1/4λϕ4+1/2g2ϕ2χ21/4 \lambda \phi^4 + 1/2 g^2\phi^2\chi^2 , where the classical oscillating inflaton field ϕ\phi decays into χ\chi-particles and ϕ\phi-particles. The parametric resonance which leads to particle production in this conformally invariant theory is described by the Lame equation. It significantly differs from the resonance in the theory with a quadratic potential. The structure of the resonance depends in a rather nontrivial way on the parameter g2/λg^2/\lambda. We construct the stability/instability chart in this theory for arbitrary g2/λg^2/\lambda. We give simple analytic solutions describing the resonance in the limiting cases g2/λ1g^2/\lambda\ll 1 and g2/λ1g^2/\lambda \gg 1, and in the theory with g2=3λg^2=3\lambda, and with g2=λg^2 =\lambda. From the point of view of parametric resonance for χ\chi, the theories with g2=3λg^2=3\lambda and with g2=λg^2 =\lambda have the same structure, respectively, as the theory 1/4λϕ41/4 \lambda \phi^4, and the theory λ/(4N)(ϕi2)2\lambda /(4 N) (\phi^2_i)^2 of an N-component scalar field ϕi\phi_i in the limit NN \to \infty. We show that in some of the conformally invariant theories such as the simplest model 1/4λϕ41/4 \lambda\phi^4, the resonance can be terminated by the backreaction of produced particles long before <χ2><\chi^2> or <ϕ2><\phi^2 > become of the order ϕ2\phi^2. We analyze the changes in the theory of reheating in this model which appear if the inflaton field has a small mass.

Keywords

Cite

@article{arxiv.hep-ph/9705347,
  title  = {Structure of Resonance in Preheating after Inflation},
  author = {Patrick Greene and Lev Kofman and Andrei Linde and Alexei Starobinsky},
  journal= {arXiv preprint arXiv:hep-ph/9705347},
  year   = {2009}
}

Comments

19 pages, revtex, 12 figures