Constraining scalar-Gauss-Bonnet Inflation by Reheating, Unitarity and PLANCK
arXiv:1606.00698 · doi:10.1103/PhysRevD.95.023514
Abstract
We revisit the inflationary dynamics in detail for theories with Gauss-Bonnet gravity coupled to scalar functions, in light of the Planck data. Considering the chaotic inflationary scenario, we constrain the parameters of two models involving inflaton-Gauss-Bonnet coupling by current Planck data. For non zero inflaton-Gauss-Bonnet coupling , an inflationary analysis provides us a big cosmologically viable region in the space of , where is the mass of inflaton. However, we study further on constraining arising from reheating considerations and unitarity of tree-level amplitude involving we have studied the constraints on arising from reheating considerations and unitarity of tree level amplitude involving graviton graviton () scattering. Our analysis, particularly on reheating significantly reduces the parameter space of for all models. he quadratic Gauss-Bonnet coupling parameter turns out to be more strongly constrained than that of the linear coupling. For the linear Gauss-Bonnet coupling function, we obtain , with the condition . However, study of the Higgs inflation scenario in the presence of Gauss-Bonnet term turned out to be strongly disfavored.
22 pages, 12 Pdf figures; Modified version including updated analyses compatible with the latest observational data. Almost matches with the published version
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