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arXiv · hep-ph/9901434

Inhomogeneity and the Post-Inflationary Universe

Richard Easther·Matthew Parry
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Abstract

We discuss the interaction between perturbations in the inflaton and the background during the preheating phase in simple inflationary models. By numerically solving the Einstein field equations we are able to assess the impact of non-linear gravitational effects on preheating, and to assess the accuracy of perturbative discussions of the preheating epoch.

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Richard Easther, Matthew Parry. 1999-01-28. Inhomogeneity and the Post-Inflationary Universe. https://doi.org/10.1063/1.59434

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