BIANCHI V COSMOLOGICAL MODEL WITH STRANGE QUARK MATTER IN f(R) GRAVITY

In this research, we have studied behaviours of quark matter and strange quark matter which exist in f(R) gravity in presence of Bianchi type uni verse. In order to obtain a deterministic solution, we have considered the scale factor which is a combination of two factors: the one is the usual power law ex pansion and the second one is an exponential function. We investigate exact f(R) functions for Bianchi V as the contribution of strange quark and quark matter. Effect of the curvature function f(R) is also observed on dynamical parameters. As per the observation both the pressure and density depend on f(R) gravity and the bag constant. Hence both $p_q$ and $\rho_q$ remain positive.