Warm (Pseudo)Scalar Inflation

Abstract

In this note, we will introduce an action for warm inflation model with direct coupling between the pseudoscalar field and mass-less $SU(2)$ 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 $\frac{{\epsilon }_{\varphi }}{1+Q}$ even in $f<M_p$ limit.

5 pages, 3 figures, 1 table, comments welcome

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