Accelerating Expansion of the Universe with Dark Matter and Holographic Dark Energy in f(T) Gravity

Kalpana Pawar¹ , N.T. Katre² , A.K. Dabre³

Section:Research Paper, Product Type: Journal-Paper
Vol.11 , Issue.2 , pp.1-9, Apr-2023

Online published on Apr 30, 2023

Copyright © Kalpana Pawar, N.T. Katre, A.K. Dabre . This is an open access article distributed under the Creative Commons Attribution License, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
 

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Abstract :
This paper deals with the study of spatially homogeneous and anisotropic Bianchi-type V space-time filled with dark matter and holographic dark energy in the framework of f(T) gravity by considering f(T)=T formalism. In order to solve the gravitational field equations completely, the exponential law of volumetric expansion has been employed. The derived cosmological model is flat and free from any kind of singularities. Some cosmologically important physical and kinematical parameters of the model have been obtained, and discussed with the help of their graphical representations. It is observed that the universe has accelerating expansion; it is stable throughout the expansion, and physically acceptable. Notably, the resultant model is consistent with the recent observations.

Key-Words / Index Term :
Bianchi-type V space-time, Anisotropy, Dark Matter, Holographic Dark Energy, Stability, f(T) Gravity.

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