English

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 SU(2)SU(2) 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 ϵϕ1+Q\frac{\epsilon_{\phi}}{1+Q} even in f<Mpf<M_p limit.

Keywords

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

R2 v1 2026-06-23T07:04:56.577Z