Higgs-Dilaton cosmology: Universality vs. criticality
arXiv:1406.5182 · doi:10.1103/PhysRevD.90.027307
Abstract
The Higgs-Dilaton model is able to produce an early inflationary expansion followed by a dark energy dominated era responsible for the late time acceleration of the Universe. At tree level, the model predicts a small tensor-to-scalar ratio (), a tiny negative running of the spectral tilt () and a nontrivial consistency relation between the spectral tilt of scalar perturbations and the dark energy equation of state, which turns out to be close to a cosmological constant (). We reconsider the validity of these predictions in the vicinity of the critical value of the Higgs self-coupling giving rise to an inflection point in the inflationary potential. The value of the inflationary observables in this case strongly depends on the parameters of the model. The tensor-to-scalar ratio can be large [] and notably exceed its tree-level value. If that happens, the running of the scalar tilt becomes positive and rather big [] and the equation-of-state parameter of dark energy can significantly differ from a cosmological constant [].
5 pages, 3 figures, published version, added clarifications and references, corrected typos
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