Bianchi type-III Cosmological Model with Linear Equation of State in f (R) Gravity

Authors

  • S. R. Bhoyar  Department of Mathematics, PhulsingNaikMahavidyalaya, Pusad, India
  • V. R. Chirde  Department of Mathematics, G. S. G. Mahavidyalaya, Umarkhed, India
  • S. H. Shekh  Department of Mathematics, J. D. Institute of Engineering & Technology, Yavatmal, India

Keywords:

Bianchi type models; linear equation of state; f(R) gravity.

Abstract

In this context, we study Bianchi type-III cosmological model with linear equation of state in the metric version of f(R) gravity. Field equations are solved by taking expansion scalar proportional to shear scalar (relation between the metric coefficients) and the law of variation of Hubble’s parameter that yields the constant value of deceleration parameter. The physical and kinematical parameters of the models have been discussed. Also, the function of the Ricci scalar is evaluated for each model.

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International Journal of Scientific Research in Science, Engineering and Technology

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Published

2017-10-31

Issue

Volume 3, Issue 6, September-October-2017

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Research Articles

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How to Cite

[1]
S. R. Bhoyar, V. R. Chirde, S. H. Shekh, " Bianchi type-III Cosmological Model with Linear Equation of State in f (R) Gravity, International Journal of Scientific Research in Science, Engineering and Technology(IJSRSET), Print ISSN : 2395-1990, Online ISSN : 2394-4099, Volume 3, Issue 6, pp.835-839, September-October-2017.