Adiabatic Gravitational Perturbation During Reheating
arXiv:hep-ph/9912510 · doi:10.1103/PhysRevD.61.121301
Abstract
We study the possibilities of parametric amplification of the gravitational perturbation during reheating in single-field inflation models. Our result shows that there is no additional growth of the super-horizon modes beyond the usual predictions.
Refs added; New version to appear in PRD
References in corpus (1)
Cited by in corpus (12)
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