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arxiv 1305.7226 v1 pith:BCN6DOSO submitted 2013-05-30 astro-ph.CO hep-th

Gauge Field Preheating at the End of Inflation

classification astro-ph.CO hep-th
keywords fieldgaugepreheatinguniverseabelianamplificationassumeconformal
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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Here we consider the possibility of preheating the Universe via the parametric amplification of a massless, U(1) abelian gauge field. We assume that the gauge field is coupled to the inflaton via a conformal factor with one free parameter. We present the results of high-resolution three-dimensional simulations of this model and show this mechanism efficiently preheats the Universe to a radiation-dominated final state.

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  1. Lectures on Reheating after Inflation

    astro-ph.CO 2019-07 unverdicted

    Lecture notes providing a generic introduction to reheating after inflation, covering its theoretical, phenomenological, and observational aspects.