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Dynamical aspects of the magnetized anisotropic cosmological model in extended gravity

  • Sankarsan Tarai
  • B. MishraEmail author
Regular Article
  • 18 Downloads

Abstract.

In this paper, we have investigated the extended gravity, in particular the f(R, T) gravity in Bianchi \(VI_{h=-1}\) space-time filled with magnetized anisotropic matter content. We have explored the field equations and obtained the solution with the power law function. The kinematical and geometrical parameters are derived and analysed in detail. The effect of energy conditions is also studied. It is found that the extended gravity, induced by \(f(R)=R\) and \(f(T)=2\Lambda_{0}+2\beta T\), where \( \Lambda_{0}\) and \(\beta\) are, respectively, the cosmological constant and coupling constant, is likely to experience an expansion at the late time of cosmic acceleration.

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Copyright information

© Società Italiana di Fisica and Springer-Verlag GmbH Germany, part of Springer Nature 2018

Authors and Affiliations

  1. 1.Department of MathematicsBirla Institute of Technology and Science-PilaniHyderabadIndia

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