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A spatially homogeneous and anisotropic Bianchi type-VI0 space-time filled with perfect fluid in general relativity and also in the framework of f ( R , T ) gravity proposed by Harko et al. (in arXiv:1104.2669 [gr-qc], 2011 ) has been studied with an appropriate choice of the function f ( R , T ). The field equations have been solved by using the anisotropy feature of the universe in Bianchi type-VI0 space time. Some important features of the models, thus obtained, have been discussed. We noticed that the involvement of new function f ( R , T ) doesn’t affect the geometry of the space-time but slightly changes the matter distribution.
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