Bianchi Type-V Space-Time with Perfect Fluid in f(R, T) Gravity

Author(s)	Dr. R.K. Dubey, Mr. Arun Kumar Tiwari
Country	India
Abstract	In this paper, we have studied Bianchi type-V space-time with perfect fluid in f(R, T) theory of gravity, where R is the Ricci scalar and T is the trace of the energy-momentum tensor . To solve gravitational field equation by using expansion anisotropy σ θ to be suitable function of average scale factor in the background of Bianchi type-V model which yields deceleration parameter is initially decelerating phase and late time accelerating phase. The kinematic and dynamical behaviour of the model have been acquired and their developments have been discussed about through their graphs. The abstract should provide a brief overview of the objectives, the Bianchi type-V model's role in understanding anisotropic universes, and how modified gravity theories provide alternatives to general relativity in explaining cosmic phenomena. It should also mention the significance of this model in addressing cosmological issues such as dark energy, dark matter, and the accelerated expansion of the universe.
Keywords	Dr.R.K.Dubey, Mr.Arun Kumar Tiwari
Field	Mathematics
Published In	Volume 7, Issue 6, November-December 2025
Published On	2025-12-26
DOI	https://doi.org/10.36948/ijfmr.2025.v07i06.63134

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