1 Department of Mathematics, Jagadamba Mahavidyalaya, Achalpur 444806, Maharashtra, India.
2 Department of Mathematics, Adarsh Science, Jairamdas Bhagchand Arts and Birla Commerce Mahavidyalaya, Dhamangaon Rly. Maharashtra 444709, India.
International Journal of Science and Research Archive, 2025, 15(03), 1209-1215
Article DOI: 10.30574/ijsra.2025.15.3.1785
Received on 27 April 2025; revised on 12 June 2025; accepted on 14 June 2025
In this paper, we investigate the Kantowski-Sachs cosmological model with a perfect fluid within the framework of Teleparallel gravity, specifically 
gravity, where 
represents the torsion scalar. The behavior of the accelerating universe is explored by adopting a specific form of 
and establishing a relationship between the metric potentials, 
. By employing the Hubble parameterization method, we derive an exact solution to the field equations that supports an accelerating universe. The physical behavior of the model is analyzed through key physical quantities, and the functional dependence of the torsion scalar on the evolution of the universe is also evaluated.
Kantowaski Sachs Universe; F(T) Theory of Gravity; Exact Solution; Cosmology
Preview Article PDF
S. C. Darunde and S. N. Bayaskar. Bulk viscous Kantowaski-Sachs Space-time with H(z) parameterization. International Journal of Science and Research Archive, 2025, 15(03), 1209-1215. Article DOI: https://doi.org/10.30574/ijsra.2025.15.3.1785.
Copyright © 2025 Author(s) retain the copyright of this article. This article is published under the terms of the Creative Commons Attribution Liscense 4.0
