Bianchi Type - III Charged Fluid Universe in Brans-Dicke Theory of Gravitation

V.G. Mete¹ , K.R. Mule² , V.M. Ingle³

Section:Research Paper, Product Type: Isroset-Journal
Vol.6 , Issue.5 , pp.57-61, Oct-2018

CrossRef-DOI:   https://doi.org/10.26438/ijsrpas/v6i5.5761

Online published on Oct 31, 2018

Copyright © V.G. Mete, K.R. Mule, V.M. Ingle . This is an open access article distributed under the Creative Commons Attribution License, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
 

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Abstract :
We investigate the spatially homogeneous Bianchi Type-III space time with electromagnetic field tensor and relativistic charged perfect fluid in Brans-Dicke (B-D) theory of gravity. Solutions have been obtained by using a general approach of solving the partial differential equations. It is observed that the convergent and isotropic solution of the metric function can be derived with the components of the vector potentials.

Key-Words / Index Term :
Bianchi type-III universe, Brans-Dicke theory of gravitation, electromagnetic field, perfect fluid, vector potentials

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