Supersymmetric Inflation with the Ordinary Higgs?
arXiv:0911.3730 · doi:10.1016/j.physletb.2010.04.049
Abstract
We consider a model of D-term inflation in which the inflaton coincides with the standard Higgs doublet. Non-renormalizable terms are controlled by a discrete R-symmetry of the superpotential. We consider radiative corrections to the scalar potential and find that Higgs inflation in the slow-roll approximation is viable and consistent with CMB data, although with a rather large value of the non-renormalizable coupling involved.
7 pages, 1 figure, published version, comments and reference added, typos and factor of 2 corrected.