1 Department of Mathematics, Shri R. R. Lahoti Science College, Morshi-444905, Dist. Amravati, M. S, India.
2 Department of Mathematics, Bapumiya Sirajoddin Patel Arts, Commerce and Science College, Pimpalgaon Kale. 443403, Dist. Buldhana M. S, India.
3 Department of Mathematics, Nabira Mahavidyalaya, Katol-441302, Dist. Nagpur, M.S, India.
International Journal of Science and Research Archive, 2023, 10(02), 1071–1079.
Article DOI: 10.30574/ijsra.2023.10.2.1070
DOI url: https://doi.org/10.30574/ijsra.2023.10.2.1070
Received on 08 November 2023; revised on 20 December 2023; accepted on 23 December 2023
In this paper we have studied minimally interacting two fluid cosmological model in the framework of scale covariant theory by considering Bianchi type III metric in the presence of matter and radiation field. Here, we have assumed the exponential volumetric law to construct this model and considered the equation of state Pm = γPm to find matter density, radiation density and parameters of matter and radiation density. Lastly, we have discussed some physical and kinematical parameters.
Bianchi Type III; Two Fluid; Scale Covariant Theory; EoS
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KN Pawar , MD Netnaskar and NT Katre. Minimally interacting two fluid cosmological model in the framework of scale covariant theory. International Journal of Science and Research Archive, 2023, 10(02), 1071–1079. https://doi.org/10.30574/ijsra.2023.10.2.1070
Copyright © 2023 Author(s) retain the copyright of this article. This article is published under the terms of the Creative Commons Attribution Liscense 4.0