An exact solution approach to warm inflation using Tsallis and Barrow holographic dark energy entropy within Rastall gravity

Abstract

This paper studies the phenomena of warm inflation in a modified cosmological scenario within Rastall gravity. In this context, we modify the standard Friedmann equations using recently proposed Tsallis and Barrow holographic dark energy entropies, alternatively. For both entropies, the exact solutions including the inflaton field, potential required to produce inflation and the scale factor are obtained under slow-roll approximation for low- and high-dissipative regimes. We obtain exponentially growing scale factors for both dark energy models. To confront the theoretical predictions of these models with recent observational data, we calculate the slow-roll parameters, number of e-folds, scalar spectral index, running of scalar spectral index and the tensor-to-scalar ratio for both extremes of dissipation. The Planck bounds on inflationary trajectories are being used to constraint the free parameters. The results are interesting and physically viable up to 2 level.

Barrow holographic dark energy in Brane world cosmology

“…Here, L is the horizon length and C is a parameter with dimension [L] −2−∆ . BHDE has been studied in different frameworks [64,65]. In the following sections, we study BHDE in a different scenario considering Hubble horizon as the IR cut-off.…”

Barrow Holographic Dark Energy in Brane World Cosmology

“…Here, L is the horizon length and C is a parameter with dimension [L] −2−∆ . Recently BHDE has been studied in different frameworks [46,47] In the following sections we study BHDE in a different scenario considering Hubble horizon as the infrared cut-off. As WMAP and other observations favours a flat universe we restrict ourselves to FRW type models with k = 0.…”