Research Article
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DOI:
http://dx.doi.org/10.24327/ijrsr.2017.0805.0276
Subject:
science
KeyWords:
Bianchi type-III space-time, f (R,T ) theory of gravity, Deceleration parameter.
Abstract:
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.