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.
Full Text 
Sign-in/Register to access full text options
Sign-in/Register to access full text options 
Published version (
Free)
Free) 
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a call
