Perfect fluid cosmological models in a modified theory of gravity

被引:0
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作者
V. U. M. Rao
K. V. S. Sireesha
D. Ch. Papa Rao
机构
[1] Andhra University,Department of Applied Mathematics
关键词
Cosmological Model; Hubble Parameter; Deceleration Parameter; Energy Momentum Tensor; Stress Energy Tensor;
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摘要
Spatially homogeneous and anisotropic Bianchi type-II, -VIII and -IX cosmological models filled with perfect fluid in the framework of the f (R, T) gravity proposed by Harko et al.(Phys. Rev. D 84, 024020 (2011)) and also in general relativity have been studied. All the models obtained and presented here are anisotropic, expanding, non-rotating and also accelerating. Some important features of the models thus obtained have been discussed. We also noticed that the involvement of the new function f (R, T) does not affect the geometry of the space-time but slightly changes the matter distribution.
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