Warm intermediate inflationary Universe model in the presence of a Generalized Chaplygin Gas

Understand

A warm intermediate inflationary model in the context of Generalized Chaplygin Gas is investigated.

• We study this model in the weak and strong dissipative regimes, considering a generalized form of the dissipative coefficient $\Gamma=\Gamma(T,\phi)$, and we describe the inflationary dynamics in the slow-roll approximation.
• We find constraints on the parameters in our model considering the Planck 2015 data, together with the condition for warm inflation $T>H$, and the conditions for the weak and strong dissipative regimes.