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Dark Energy Scenario in Metric f(R) Formalism

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Abstract

Friedmann–Robertson–Walker (FRW) space–time with bulk viscosity in the context of f(R) gravity is considered. The field equations are solved for the Power and Exponential volumetric expansion. Two types of functional relationship i.e. f(R) = R + bRm and \( \,f(R) = R - \frac{{\lambda^{4} }}{R} \) are investigated. The Phantom, Chaplygin gas and Tachyon fields are discussed. It is observed that the universe is open and inflationary.

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Acknowledgements

The authors would like to thank the anonymous referees for giving very enlightening and constructive suggestions which helped in improving the manuscript.

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Authors and Affiliations

  1. Department of Mathematics, Sant Gadge Baba Amravati University, Amravati, 444602, India

    S. D. Katore

  2. Department of Mathematics, A.E.S. Art Commerce and Science College, Hingoli, 431513, India

    S. P. Hatkar

  3. Department of Mathematics, Prof. Ram Meghe Institute of Technology and Research, Badnera, India

    P. S. Dudhe

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  1. S. P. Hatkar
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Hatkar, S.P., Dudhe, P.S. & Katore, S.D. Dark Energy Scenario in Metric f(R) Formalism. Found Phys 49, 1067–1085 (2019). https://doi.org/10.1007/s10701-019-00302-x

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