Research Article | Open Access | Download PDF
Volume 69 | Issue 8 | Year 2023 | Article Id. IJMTT-V69I8P505 | DOI : https://doi.org/10.14445/22315373/IJMTT-V69I8P505
Interacting Tsallis Holographic Dark Energy Models
with Constant Deceleration Parameter
Vaibhav D. Bokey
| Received |
Revised |
Accepted |
Published |
| 13 Jun 2023 |
28 Jul 2023 |
10 Aug 2023 |
25 Aug 2023 |
Abstract
In this work, we investigate an anisotropic and homogeneous Bianchi Type-I universe filled with Dark Matter
(DM) and Dark Energy (DE) in the framework of Einstein’s theory of Relativity. We choose an interaction between DM and
DE with the interacting term,𝑄 = 3𝐻𝛾𝜌𝑚, by considering Tsallis generalized entropy. The exact solutions of the field
equations are obtained by using the laws of the Hubble parameter proposed by Berman [1]. The EoS parameter of Tsallis
Holographic DE (THDE) is explaining the evolution of the universe as The EoS parameter is Phantom like, Quintessence
like and approaches to ΛCDM model. The EoS parameter, Anisotropy Parameter, Deceleration parameter, Total Energy
Density parameter are explained by graphical representation in both models. The results, we obtained are consistent with
the observational data.
Keywords
Tsallis holographic dark energy, Bianchi-I Universe, Constant deceleration parameter, General relativity.
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Citation :
Vaibhav D. Bokey, "Interacting Tsallis Holographic Dark Energy Models
with Constant Deceleration Parameter," International Journal of Mathematics Trends and Technology (IJMTT), vol. 69, no. 8, pp. 36-44, 2023. Crossref, https://doi.org/10.14445/22315373/IJMTT-V69I8P505
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