\begin{document}$\Gamma(\phi,T)= C_{\phi} {T^{a}}/{\phi^{a-1}}$\end{document}, where \begin{document}$C_{\phi}$\end{document} is a dimensionless parameter and a is the inflation decay rate. In a scenario where our model operates within a robust dissipative environment \begin{document}$(R\gg1)$\end{document}, we analyze both fundamental and perturbative dynamics to extract key inflationary parameters. These include the scalar power spectrum \begin{document}${{\cal{P}}_{{\cal{R}}}}$\end{document}, dissipative ratio R, scalar spectral index \begin{document}$n_{s}$\end{document}, tensor-to-scalar ratio r, running of the scalar spectral index \begin{document}$\dfrac{{\rm d}n_{s}}{{\rm d}\ln{k}}$\end{document}, and generalized ratio of the swampland de-Sitter conjecture \begin{document}$\dfrac{T'V}{V'T}$\end{document} for three different potentials."> Chaplygin gas inspired warm inflation and swampland conjectures through various scalar potentials -
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