Issues in Palatini inflation: Bounds on the Reheating Temperature
arXiv:2210.00837 · doi:10.1103/PhysRevD.106.123530
Abstract
We consider -inflation in Palatini gravity, in the presence of scalar fields coupled to gravity. These theories, in the Einstein frame, and for one scalar field , share common features with - inflation models. We apply this formalism for the study of single-field inflationary models, whose potentials are monomials, , with a positive even integer. We also study the Higgs model non-minimally coupled to gravity. With -terms coupled to gravity as , with constant, the instantaneous reheating temperature , is bounded by , with the upper bound being saturated for large . For such large need go beyond slow-roll to calculate reliably the cosmological parameters, among these the end of inflation through which is determined. In fact, as inflaton rolls towards the end of inflation point, the quartic in the velocity terms, unavoidable in Palatini gravity, play a significant role and can not be ignored. The values of , and other parameters, are constrained by cosmological data, setting bounds on the inflationary scale and the reheating temperature of the Universe.
35 pages, 18 figures, PDFLaTeX, text and references added, typos corrected
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