Tachyon Warm-Intermediate Inflationary Universe Model in High Dissipative Regime

Understand

We consider tachyonic warm-inflationary models in the context of intermediate inflation.

• We derive the characteristics of this model in slow-roll approximation and develop our model in two cases, 1- For a constant dissipative parameter $\Gamma$.
• 2- $\Gamma$ as a function of tachyon field $\phi$.
• We also describe scalar and tensor perturbations for this scenario.