  The warm inflationary scenario is investigated in the context of affine
gravity formalism. A general framework is provided for studying different
single-field potentials. Using the sphaleron mechanism we explain the
continuous dissipation of the inflaton field into radiation, leading to the
$\Gamma=\Gamma_0 T^3$ dissipation coefficient. The treatment is performed in
the weak and strong dissipation limits. We consider the quartic potential as a
case study to provide a detailed study. Moreover, in this study, we discuss
various constraints on inflationary models in general. We compare the
theoretical results of the quartic potential model within warm inflation with
the observational constraints from Planck $2018$ and BICEP/Keck 2018, as
presented by the tensor-to-scalar ratio, spectral index and the perturbation
spectrum.
