Anisotropic Bianchi type VI<sub>0</sub> Space-Time with Barotropic Fluid in Sáez - Ballester Theory of Gravitation

Authors

  • P. Kumawat Department of Mathematics, Swami Keshvanand Institute of Technology, Management & Gramothan, Jaipur-302017, India
  • R. Goyal Department of Mathematics, S. S. Jain Subodh PG College, Jaipur, India
  • S. Choudhary Department of Mathematics, Swami Keshvanand Institute of Technology, Management & Gramothan, Jaipur-302017, India

DOI:

https://doi.org/10.3329/jsr.v16i3.70809

Abstract

In this paper, we have discussed the exact solution of Einstein's field equations for anisotropic Bianchi type VI0 cosmological model in the framework of the scalar-tensor theory of gravitation given by Sáez–Ballester for barotropic fluid distribution. To obtain an exact solution, we have assumed that expansion (θ) is proportional to shear (σ) which leads to A =Bk, where k is a constant A and B are metric potentials and also assumed barotropic condition p = γρ; (0 ≤ γ ≤ 1) where p being isotropic pressure and ρ is matter density. Some physical and geometrical properties of the model are also discussed.

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Published

2024-09-02

How to Cite

Kumawat, P., Goyal, R., & Choudhary, S. (2024). Anisotropic Bianchi type VI<sub>0</sub> Space-Time with Barotropic Fluid in Sáez - Ballester Theory of Gravitation. Journal of Scientific Research, 16(3), 695–703. https://doi.org/10.3329/jsr.v16i3.70809

Issue

Vol. 16 No. 3 (2024)

Section

Section A: Physical and Mathematical Sciences

License

Creative Commons License

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© Journal of Scientific Research

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