Study of warm inflationary models and their parameter estimation from CMB

Warm inflation is a natural and well-motivated description of cosmic inflation which accounts for the inflaton dissipation and radiation production during the inflationary phase, neglected in the standard cold description. It results in crucial differences in the imprints on the Cosmic Microwave Background (CMB) radiation from the standard cold description. In this study, we consider warm inflation models with λφ4 and λφ6 potentials and estimate their model parameters consistent with CMB using the CosmoMC numerical code. These models are characterized by the inflaton self coupling, λ, and the dissipation parameter, QP, due to the inflaton's dissipation into the other fields. Therefore, information about these physical parameters is essential from the perspective of the model building. In our analysis, we also calculate the spectral index, ns, and the tensor-to-scalar ratio, r, for the mean values of the parameters and show that for the weak dissipative regime, r, is within the sensitivity of the next generation CMB polarization experiments, which is an important observational test for these models.