Warm-polytropic inflationary universe model

In the present paper we study warm inflationary universe models in the context of a polytropic gas. We derive the characteristics of this model in slow-roll approximation and develop our model in two cases, 1- For a constant dissipative parameter $\mathrm{\Gamma }$. 2- $\mathrm{\Gamma }$ as a function of scalar field $\varphi$. In these cases we will obtain exact solution for the scalar field and Hubble parameter. We will also obtain explicit expressions for the tensor-scalar ratio $R$, scalar spectrum index $n_s$ and its running ${\alpha }_s$, in slow-roll approximation.