Magnetized Bianchi type III anti-stiff fluid consmological models with time dependent Λ and variable magnetic permeability
1Department of Mathematics Pacific institute of Engineering Pacific Academy of Higher education and Research University Udaipur: 313024 (INDIA)
2Department of Mathematics and Statistics, University College of Science Mohanlal Sukhadia University, Udaipur: 313001 (INDIA)
E-mail: gajendrasingh237@gmail.com, E-mail: tyagi.atul10@gmail.com
The behavior of cosmological constant in homogeneous Bianchi type-III universe is investigated for magnetized anti-stiff perfect fluid distribution. The magnetic permeability is assumed as a variable quantity. The magnetic field is due to an electric current produce along x- axis, thus F23 is the only non vanishing component of electromagnetic field tensor. For the complete determination of the model we assume a condition between metric potential A = Cn. Physical and Geometrical features of model in presence and absence of magnetic field are also discussed.
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1GAJENDRA PAL SINGH and 2ATUL TYAGI, "Magnetized Bianchi type III anti-stiff fluid consmological models with time dependent Λ and variable magnetic permeability", Journal of Ultra Scientist of Physical Sciences, Volume 24, Issue 2, Page Number , 2016Copy the following to cite this URL:
1GAJENDRA PAL SINGH and 2ATUL TYAGI, "Magnetized Bianchi type III anti-stiff fluid consmological models with time dependent Λ and variable magnetic permeability", Journal of Ultra Scientist of Physical Sciences, Volume 24, Issue 2, Page Number , 2016Available from: https://www.ultrascientist.org/paper/422/
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