Consequences of Holographic Dark Energy Cosmological Model in Gravity

Authors

  • S. H. Shekh Department of Mathematics, S.P.M. Science and Gilani Arts and Commerce College, Ghatanji-445301, India
  • V.R. Chirde Department of Mathematics, G. S. G. Mahavidyalaya, Umarkhed-445206, India
  • S. Raut Department of Mathematics, PLITMS, Buldhana-443001, India

DOI:

https://doi.org/10.37256/cm.11201951

Keywords:

Bianchi typespace-time, holographic dark energy, gravity

Abstract

We have investigated the dynamics of spatially homogeneous Bianchi type-I (LRS) space-time filled with two minimally interacting fields-matter and holographic dark energy components with volumetric power laws expansion towards the gravitational field equations of the linear form of gravity. Solving the set of field equation, we obtained the exact solution and observed that the mode of expansion of the model is accelerating throughout the evolution due to destructive assessment of deceleration parameter. Also, it has found that the Gauss-Bonnet invariant and the function of Gauss-Bonnet invariant both are not occur for, the equation of state parameter admits the different values for different values of n which are relevant in the standard range provided by recent theoretical and experimental data along with the model has a Big-Bang type of singularity at singular point.

Author Biography

S. H. Shekh, Department of Mathematics, S.P.M. Science and Gilani Arts and Commerce College, Ghatanji-445301, India

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Published

2019-10-21

How to Cite

1.
S. H. Shekh, V.R. Chirde, S. Raut. Consequences of Holographic Dark Energy Cosmological Model in Gravity. Contemp. Math. [Internet]. 2019 Oct. 21 [cited 2024 Mar. 29];1(1):45-53. Available from: https://ojs.wiserpub.com/index.php/CM/article/view/cm.11201951.49-57