A Study on Homogenous cosmological model in f (R, T) Theory of gravity

Authors

  • Vandana Soni & Sudha Agrawal

Keywords:

Bianchi Type-V cosmological models, f (R, T) Theory of gravity, Deceleration parameter, Bulk viscous fluid, Scale Factor Evolution, Field Equations, Cosmological Solutions and properties

Abstract

This study introduces non-singular Bianchi type I and V cosmological models together with aspecific value for the average scale factor, related to a time-dependent deceleration parameter.The cosmological models first demonstrate acceleration for a limited period before shifting todeceleration. The physical and kinematic properties of the universe models are analyzed.

References

A. K. Yadav. Cosmological constant dominated transit universe from the early deceleration phase to the current acceleration phase in Bianchi-V Spacetime, Chin. Phys. Lett. 2012, Vol.29 Issue 7 9801.

A.G. Riess et al. BV RI LIGHT curves for 22 Type Ia supernovae, The astrophysical journal 1998, Vol. 116, 1009

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Published

2024-09-23

How to Cite

Vandana Soni & Sudha Agrawal. (2024). A Study on Homogenous cosmological model in f (R, T) Theory of gravity. Journal of Computational Analysis and Applications (JoCAAA), 33(06), 2123–2133. Retrieved from https://eudoxuspress.com/index.php/pub/article/view/3010

Issue

Vol. 33 No. 06 (2024): JOCAAA

Section

Articles

License

Creative Commons License

This work is licensed under a Creative Commons Attribution 4.0 International License.