Dark Energy and Tachyon Field in Bianchi Type-V Space-time

Abstract

In this paper, we consider Bianchi type-V space-time and study a cosmological model of dark energy based on Tachyon scalar field. We assumed three different kinds of matter without possibility of interaction with scalar dark energy. Assuming power law Hubble parameter in terms of scale factor we obtain evolution of scalar field, scalar potential and equation of state parameter.

arXiv comment18 pages

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• Stability and interacting $f(T,\mathcal{T})$ gravity with modified Chaplygin gas
• Cosmological Tests of $f(R,G,T)$ Dark Energy Model in FRW Universe
• Observational constraints and stability in viscous $f(T,\mathcal{T})$ gravity
• Viscous interacting and stability on dark matter Bose-Einstein condensation with modified Chaplygin gas