Anisotropic Barrow Holographic Dark Energy Models in Scalar-Tensor Theory of Gravitation

  • Y. Sobhanbabu SRKR Engineering College (A), Bhimavaram, India https://orcid.org/0000-0003-0717-1323
  • G. Satyanarayana Sasi Institute of Technology and Engineering College (A), Tadepalligudem, India
  • N.V.S. Swamy Chinamilli SRKR Engineering College (A), Bhimavaram, India
  • P.V. Rambabu SRKR Engineering College (A), Bhimavaram, India
DOI: https://doi.org/10.26565/2312-4334-2024-2-04
Keywords: Bianchi type-III Universe, Сosmology, Saez-Ballester theory

Abstract

In this research, we have derived the solution of the field equations of the scalar-tensor theory of gravitation, proposed by Saez and Ballester(Phys. Lett. A113, 467:1986) within the frame-work of Bianchi type-III Universe. We have analyzed the interacting and non-interacting anisotropic Barrow Holographic Dark Energy (BHDE) models by assuming the time dependent deceleration parameter q(t). Further, we have discussed the several cosmological parameters such as energy densities of pressureless dark matter and BHDE, skewness, deceleration, equation of state parameters, ωBH-ω'BH plane and stability of the both interacting and non-interacting models. Also, we have observed that in our non-interacting and interacting models deceleration and equation of state parameters support the recent observational data.

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Published
2024-05-18
Cited
How to Cite
Sobhanbabu, Y., Satyanarayana, G., Chinamilli, N. S., & Rambabu, P. (2024). Anisotropic Barrow Holographic Dark Energy Models in Scalar-Tensor Theory of Gravitation. East European Journal of Physics, (2), 48-63. https://doi.org/10.26565/2312-4334-2024-2-04
Issue
No. 2 (2024): East European Journal of Physics
Section
Original Papers

Copyright (c) 2024 Y. Sobhanbabu, G. Satyanarayana, N.V.S. Swamy Chinamilli, P.V. Rambabu

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