Magnetized Anisotropic Dark Energy Bianchi Type III Cosmological Models in Brans-Dicke Theory of Gravitation

Authors

  • V.B. Raut Department of Mathematics, S.G.B. Amravati University, Amravati-444602, India
  • K.S. Adhav Department of Mathematics, S.G.B. Amravati University, Amravati-444602, India
  • S.D. Katore Department of Mathematics, S.G.B. Amravati University, Amravati-444602, India
  • N.K. Sarkate Department of Mathematics, S.G.B. Amravati University, Amravati-444602, India

DOI:

https://doi.org/10.15379/2408-977X.2014.01.02.5

Keywords:

Bianchi Type III Universe, Brans-Dicke Theory of Gravitation, Dark Energy.

Abstract

We investigate the spatially homogeneous Bianchi Type III cosmological models with magnetized anisotropic dark energy fluid in the scalar tensor theory of gravitation proposed by Brans-Dicke [1]. The solutions of the models are obtained by volumetric exponential expansion, power law expansion and power law relation between scalar field and scale factor ‘a’. The physical aspects of the dark energy models are discussed.

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Published

2014-12-31

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Vol. 1 No. 2 (2014)

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