Journal
ASTROPHYSICS AND SPACE SCIENCE
Volume 342, Issue 1, Pages 249-252Publisher
SPRINGER
DOI: 10.1007/s10509-012-1158-7
Keywords
f(R, T) gravity; Bianchi type-III model; Hubble's parameter
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A spatially homogeneous Bianchi type-III space-time is considered in the presence of perfect fluid source in the frame work of f(R,T) gravity (Harko et al. in Phys. Rev. D 84:024020, 2011) with the help of a special law of variation for Hubble's parameter proposed by Bermann (Nuovo Cimento B 74:182, 1983). A cosmological model with an appropriate choice of the function f(T) has been constructed. The physical behavior of the model is studied.
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