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Bianchi Type-V space time with Tsallis holographic dark energy

A. Narasimharao

https://orcid.org/0009-0001-8833-2338

Department of Mathematics, GITAM (Deemed to be University), Visakhapatnam, Andhrapradesh 530 045, India

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and

D. Neelima

https://orcid.org/0000-0003-1625-5596

Department of Mathematics, GITAM (Deemed to be University), Visakhapatnam, Andhrapradesh 530 045, India

E-mail Address: neeludavuluri@gmail.com

Corresponding author.

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https://doi.org/10.1142/S0219887824500634Cited by:0 (Source: Crossref)

Abstract

In this paper, using the framework of Saez–Ballester theory, Bianchi Type-V metric Tsallis holographic dark energy models with interacting and non-interacting elements have been constructed. To obtain solutions for the model, we used correlation between metric potentials and varying deceleration parameters. There is additional discussion of the models’ physical characteristics and behavior.

Keywords:

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