Warm (Pseudo)Scalar Inflation
General Relativity and Quantum Cosmology
2019-08-21 v1
Abstract
In this note, we will introduce an action for warm inflation model with direct coupling between the pseudoscalar field and mass-less gauge fields. The potential of inflaton is protected against the thermal corrections in a thermal bath of gauge fields even with strong direct interaction between inflaton and light fields. The dissipation parameter of this model is approximately constant in the high-dissipative regime. In this regime, the model is compatible with observational data and non-Gaussianity is in order of Hubble slow-roll parameter even in limit.
Cite
@article{arxiv.1901.01897,
title = {Warm (Pseudo)Scalar Inflation},
author = {Vahid. Kamali},
journal= {arXiv preprint arXiv:1901.01897},
year = {2019}
}
Comments
5 pages, 3 figures, 1 table, comments welcome