Magnetized strange quark matter in reconstructedf(R;T)gravity for Bianchi Iand V universes with cosmological constant

Abstract

In this article, we have investigated the behaviors of magnetized strange quark matter distributions for BianchiI and V universes in reconstructedf(R;T) =1R+2f3(T) gravity (here1and2are constants;f3(T) is an arbitraryfunction ofT). To get solutions of the eld equations we have used a deceleration parameter and the equation of statefor strange quark matter. The new representedf(R;T) model includes two models of Harko et al. and transforms togeneral relativity. Whent! 1, we get the dark energy model (p= ) in reconstructedf(R;T) =1R+2f3(T)gravity. However, we obtain zero magnetic eld in allf(R;T) gravitation models.