Breakdown of the semiclassical approximation during the early stages of preheating
Paul R. Anderson, Carmen Molina-Paris, and Dillon H. Sanders

TL;DR
This paper investigates the limits of the semiclassical approximation during early preheating in chaotic inflation models, showing it breaks down before scattering or backreaction effects become significant.
Contribution
It introduces a modified criterion for the validity of the semiclassical approximation and demonstrates its failure during the initial stages of preheating.
Findings
Semiclassical approximation breaks down early in preheating
Large fluctuations in quantum field two-point functions occur
Validity criterion predicts breakdown before scattering effects
Abstract
The validity of the semiclassical approximation is investigated during the preheating phase in models of chaotic inflation using a modification of a criterion previously proposed for semiclassical gravity. If the modified criterion is violated then fluctuations of the two-point function for the quantum fields are large and the semiclassical approximation is not valid. Evidence is provided that the semiclassical approximation breaks down during the early stages of preheating, well before either scattering effects or backreaction effects are important.
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