Note on the reheating temperature in Starobinsky-type potentials
General Relativity and Quantum Cosmology
2021-04-14 v3
Abstract
The relation between the reheating temperature, the number of e-folds and the spectral index is shown for the Starobinsky model and some of its descendants through a very detailed calculation of these three quantities. The conclusion is that for viable temperatures between MeV and GeV the corresponding values of the spectral index enter perfectly in its C.L., which shows the viability of this kind of models.
Keywords
Cite
@article{arxiv.2005.14653,
title = {Note on the reheating temperature in Starobinsky-type potentials},
author = {Jaume Haro and Llibert Aresté Saló},
journal= {arXiv preprint arXiv:2005.14653},
year = {2021}
}
Comments
Version accepted for publication in GERG