Bianchi Type- III Perfect Fluid Dark Energy Cos- mological Model with Dynamical Equation of State Parameter in f(R,T) Theory of Gravity

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DOI : https://doi.org/10.56424/jts.v18i01.221
Published Feb 3, 2025

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Priyanka Kumari
Rajkiya Engineering College Chandpur Bijnor
S Ram
IIT BHU Varanasi
K S Adhav
Department of Mathematics ,Sant Gadge Baba Amravati University , Amravati(India)444602

Abstract

We investigate some spatially homogeneous
Bianchi type-III dark energy cosmological model with equation
of state parameter in presence of perfect fluid within
the framework of modified f(R,T) gravity theory with the
help of special form of deceleration parameter for FRW
metric proposed by Singh and Debnath [1] . We have also
assumed that the scalar expansion is proportional to the
shear and the EoS parameter is proportional to skewness
parameter in this model. Some physical and kinematical
behaviour of the model are also discussed in detail .

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How to Cite
Kumari, P., Ram, S., & Adhav, K. S. (2025). Bianchi Type- III Perfect Fluid Dark Energy Cos- mological Model with Dynamical Equation of State Parameter in f(R,T) Theory of Gravity. Journal of the Tensor Society, 18(01), 09-18. https://doi.org/10.56424/jts.v18i01.221
Issue
Vol 18 No 01 (2024): Journal of the Tensor Society
Section
Articles
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Author Biography

S Ram, IIT BHU Varanasi

Department of Mathematics IIT (BHU) Varansi 221005,
India

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