Skip to main content
Log in

Bianchi type VI h perfect fluid cosmological model in f(R,T) theory

  • Original Article
  • Published:
Astrophysics and Space Science Aims and scope Submit manuscript

Abstract

In this paper, we have investigated Bianchi type VI h cosmological model filled with perfect fluid in the framework of f(R,T) gravity, where R is the Ricci scalar and T is the trace of the energy-momentum tensor proposed by Harko et al. (Phys. Rev. D 84:024020, 2011). We have obtained the cosmological models by solving the field equations. Some physical behaviors of the model are also studied.

This is a preview of subscription content, log in via an institution to check access.

Access this article

Price excludes VAT (USA)
Tax calculation will be finalised during checkout.

Instant access to the full article PDF.

Similar content being viewed by others

References

Download references

Acknowledgements

BM acknowledges University Grants Commission, New Delhi, India for financial support to carry out the Minor Research Project [F.No. 42-1001/2013(SR)].

The authors are very much thankful to the honorable referee for the valuable comments and suggestions for the improvement of the paper.

Author information

Authors and Affiliations

Authors

Corresponding author

Correspondence to B. Mishra.

Rights and permissions

Reprints and permissions

About this article

Cite this article

Mishra, B., Sahoo, P.K. Bianchi type VI h perfect fluid cosmological model in f(R,T) theory. Astrophys Space Sci 352, 331–336 (2014). https://doi.org/10.1007/s10509-014-1914-y

Download citation

  • Received:

  • Accepted:

  • Published:

  • Issue Date:

  • DOI: https://doi.org/10.1007/s10509-014-1914-y

Keywords

Navigation