Perfect Fluid Bianchi-Iii Cosmological Model In F(R,T) Gravity

The spatially homogeneous & anisotropic Bianchi-III cosmological model in the presence of perfect fluid within the framework of f (R,T ) gravity is investigated. To get the exact solution of Einstein’s field equations we have taken a special form of deceleration parameter and also used b C = V ^b where C is metric coefficient, V is volume scale factor and b is any constant. The behavior of the important parameters like expansion scalar, shear scalar and average anisotropy parameter is discussed in detail.