Role of Relativistic Charged Perfect Fluid in Bianchi type-III Space-time in Brans-Dicke theory of gravitation

V. G.Mete 1, *, K. R.Mule 2, S. N. Bayaskar 3 and V.S. Bawane 4

1 Department of Mathematics, R.D.I.K. & K.D. College, Badnera-Amravati-444701, India.
2 Department of Mathematics, S. D. M. Burungale Science and Arts College, Shegaon-444203, India.
3 Department of Mathematics, Adarsha Science, J. B. Art and Birla Commerce College, Dhamangaon Rly- 444709, India.
4 Department of Mathematics, M. F. Arts, Comm. & S. C. Science Mahavidyalaya, Warud-444906, India
 
Review
International Journal of Science and Research Archive, 2024, 11(02), 035–044.
Article DOI: 10.30574/ijsra.2024.11.2.0355
Publication history: 
Received on 13 January 2024; revised on 24 February 2024; accepted on 27 February 2024
 
Abstract: 
In this paper, we investigate the role of relativistic charged perfect fluid in Bianchi type-III cosmological model in Brans-Dicke theory of gravitation. Solutions of the model are obtained by volumetric exponential expansion, power law expansion and power law relation between scalar field  and the scale factor . Some physical and kinematical properties of the model also are studied.
 
Keywords: 
Bianchi type-III universe; Brans-Dicke theory of gravitation; Electromagnetic field; Perfect fluid; Constant vector potentials
 
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