Preheating in Palatini Higgs inflation

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Published 12 April 2019 © 2019 IOP Publishing Ltd and Sissa Medialab
, , Citation Javier Rubio and Eemeli S. Tomberg JCAP04(2019)021 DOI 10.1088/1475-7516/2019/04/021

1475-7516/2019/04/021

Abstract

We study the details of preheating in Palatini Higgs inflation. We show, that contrary to what happens in the metric formulation of the model, the Universe does not reheat through the creation of gauge bosons only, but also through the tachyonic production of Higgs excitations. The latest entropy production channel turns out to be very efficient and leads to an almost instantaneous onset of radiation domination after the end of inflation. As compared to the metric case, this reduces the number of e-folds needed to solve the usual hot big bang problems while leading to a smaller spectral index for the primordial spectrum of density perturbations.

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10.1088/1475-7516/2019/04/021