Magnetized bulk viscous Bianchi type ix cosmological models with variable A
Author & Affiliation:
ATUL TYAGI
Department of Mathematics & Statics, University, College of Science, Mohanlal Sukhadia, University, Udaipur - 313001 (INDIA)
GAJENDRA PAL SINGH (gajendrasingh237@gmail.com0
Department of Mathematics Maharaja College of Engineering Udaipur - 313024 (INDIA)
Keyword:
Bianchi IX, Electromagnetic field, Bulk Viscous fluid, Variable
Issue Date:
August 2010
Abstract:
Some Bianchi type IX cosmological models with electromagnetic field are investigated in presence of bulk viscous fluid. For the complete determination of the model we assume that expansion (¢) in the model is proportional to the eigen value of the shear tensorThis condition leads to where and n are constants. Also the fluid obey the equation of state p = rg where 0 £ g £ 1. Some physical and geometrical features of the models are also discussed.
Pages:
658-664
ISSN:
2319-8044 (Online) - 2231-346X (Print)
Source:
PDF:
DOI:
jusps-A
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Copy the following to cite this article:
A. Tyagi; G. P. Singh, "Magnetized bulk viscous Bianchi type ix cosmological models with variable A", Journal of Ultra Scientist of Physical Sciences, Volume 22, Issue 2, Page Number 658-664, 2018Copy the following to cite this URL:
A. Tyagi; G. P. Singh, "Magnetized bulk viscous Bianchi type ix cosmological models with variable A", Journal of Ultra Scientist of Physical Sciences, Volume 22, Issue 2, Page Number 658-664, 2018Available from: https://www.ultrascientist.org/paper/1017/
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