Analysis shows polarisation and temperature CMB data constrain axion warm inflation parameters, highlighting key dynamics.
Axion warm inflation is studied within the framework of Logamediate inflation. Using a novel approach, we constrain the parameter space of the model and find a reasonable region of free parameters compatible with the temperature, polarization, and lensing CMB data. We focus on an inflaton evolution characterized by a high dissipative regime, where particle production impacts the inflaton dynamics more than the expansion rate. Specifically, we consider the cubic form of the dissipation coefficient, Υ=Υ0T3, as proposed in minimal warm inflation. We show that this parameter remains large during the slow-roll epoch for a broad range of the free parameter Υ0, as indicated by our data analysis.
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Shamloui et al. (2025) studied this question.
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