Bianchi type-III cosmological model in f(R,T) theory of gravity

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 7...

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Published inAstrophysics and space science Vol. 342; no. 1; pp. 249 - 252
Main Authors Reddy, D. R. K., Santikumar, R., Naidu, R. L.
Format Journal Article
LanguageEnglish
Published Dordrecht Springer Netherlands 01.11.2012
Springer Nature B.V
Subjects
Astrobiology
Astronomy
Astrophysics
Astrophysics and Astroparticles
Cosmology
Gravity
Mathematical models
Observations and Techniques
Original Article
Physics
Physics and Astronomy
Space Exploration and Astronautics
Space Sciences (including Extraterrestrial Physics
(
Hubble’s parameter
Bianchi type-III model
,
gravity
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Summary: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.
Bibliography:ObjectType-Article-1
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ISSN:0004-640X
1572-946X
DOI:10.1007/s10509-012-1158-7