Abstract
Abstract
In this paper, Bianchi type-V cosmological model in perfect fluid with quadratic equation of state p= αρ2-ρ, where α≠ 0, has been studied in modified theory of gravity. The general solution of the f(R, T) equations for Bianchi type-V space-time has been obtained by considering a law of variation of scale factor which yields a time dependent deceleration parameter. The model represents the transition of the universe from early deceleration phase to the recent accelerated expansion phase.
Subject
General Physics and Astronomy
Cited by
1 articles.
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1. Exploring $$f\left(R,T\right)$$ Theory with Polytropic Equation of State;International Journal of Applied and Computational Mathematics;2023-12-16