Minimal higgs inflation

Abstract

We consider a possibility that the Higgs field in the Standard Model (SM) serves as an inflaton when its value is around the Planck scale. We assume that the SM is valid up to an ultraviolet cutoff scale wedge;, which is slightly below the Planck scale, and that the Higgs potential becomes almost flat above wedge;. Contrary to the ordinary Higgs inflation scenario, we do not assume the huge non-minimal coupling, of O(104), of the Higgs field to the Ricci scalar. We find that wedge; must be less than 5 × 1017 GeV in order to explain the observed fluctuation of the cosmic microwave background, no matter how we extrapolate the Higgs potential above wedge;. The scale 10 17 GeV coincides with the perturbative string scale, which suggests that the SM is directly connected with string theory. For this to be true, the top quark mass is restricted to around 171 GeV, with which wedge; can exceed 1017 GeV. As a concrete example of the potential above wedge;, we propose a simple log-type potential. The predictions of this specific model for the e-foldings N* = 50-60 are consistent with the current observation, namely, the scalar spectral index is ns = 0.977-0.983 and the tensor to scalar ratio 0 < r < 0.012-0.010. Other parameters, dn s/d ln k, nt , and their derivatives, are also consistent. © The Author(s) 2014.