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Gauge Field Preheating at the End of Inflation

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.

preprint2013arXivOpen access
J. Tate DeskinsJohn T. Giblin JrRobert R. Caldwell
astro-ph.COhep-th
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J. Tate DeskinsJohn T. Giblin JrRobert R. Caldwell

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