Post-inflationary Scalar Tensor Cosmology and Inflationary Parameters

Abstract

Scalar fields provide attractive modifications of pre-BBN cosmology, which have interesting implications for dark matter abundances. We analyse the effect of these modifications on the number of e-foldings between horizon exit of CMB modes and the end of inflation $(N_k)$, and examine the consequences for inflationary predictions of various models. We find significant effects in the predictions in the $(n_s,r)$ plane. For a large part of the parameter space, the shift in $N_k$ is positive; this ameliorates the tension of $m^2\ddot{I}{†}^2$ and natural inflation with data.

19 pages, 2 figures. References added, minor changes. Version to appear in PRD