Preheating and Thermalization after Inflation

Abstract

After a short review of inlationary preheating, we discuss the development of equilibrium in the frameworks of massless λ 4 model. It is shown that the process is characterised by the appearance of Kolmogorov spectra and the evolution towards thermal equilibrium follows self-similar dynamics. Simplified kinetic theory gives values for all characteristic exponents which are close to what is observed in lattice simulations. This allows estimation of the resulting reheating temperature.

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