Warm intermediate inflationary Universe model in the presence of a Generalized Chaplygin Gas
Abstract
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 =(T,φ), 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.
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