Renyi Holographic Dark Energy Model in f(R) Gravity with Hubble's IR Cut-Off

Authors

DOI:

https://doi.org/10.26565/2312-4334-2023-3-06

Keywords:

f(R) Gravity, RHDE, dark matter, Cosmology, Bianchi type-I space-time

Abstract

In the present study, a homogeneous and anisotropic LRS Bianchi type-I universe model is considered with an interacting dark matter and Renyi holographic dark energy model (RHDE) in f(R) gravity. The deceleration parameter (DP) shows a signature flipping for a universe which was decelerating in past and accelerating at present epoch. Therefore, the DP is a most physically justified parameter to analyze the solution of cosmological model. In order to find an exact solution of the field equations of the model, the shear scalar is considered to be proportional to the expansion scalar. We have considered f(R) = b Rn, the depiction model of f(R) which is the function of Ricci scalar R. The physical and geometrical characteristics of the universe model have been studied.

Author Biographies

  • Kishor S. Wankhade, Department of Mathematics, Yashwantrao Chavan Arts and Science Mahavidyalaya, Mangrulpir Dist. Washim, India

    Assistant Professor, Department of Mathematics

  • Alfred Y. Shaikh, Department of Mathematics, Indira Gandhi Mahavidyalaya, Ralegaon, India

    Assistant Professor, Department of Mathematics

  • Siraj N. Khan, Prof. Ram Meghe College of Engineering and Management, Badnera, Amravati, India

    Assistant Professor, Department of Mathematics

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Published

2023-09-04

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No. 3 (2023): East European Journal of Physics

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Original Papers

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How to Cite

Renyi Holographic Dark Energy Model in f(R) Gravity with Hubble’s IR Cut-Off. (2023). East European Journal of Physics, 3, 87-95. https://doi.org/10.26565/2312-4334-2023-3-06

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