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Journal of Ultra Scientist of Physical Sciences - A
Voulume: 35
Issue: 7
Article No. 1
Bianchi Type-VIII Inflationary Cosmological Models with Flat Potential and Stiff perfect Fluid Distribution in General Relativity
DHIRENDRA CHHAJED
Department of Mathematics and Statistics, University College of Science, Mohanlal Sukhadia University, Udaipur-313001 Rajasthan (INDIA)
MONIKA
Department of Mathematics and Statistics, University College of Science, Mohanlal Sukhadia University, Udaipur-313001 Rajasthan (INDIA)
ATUL TYAGI
Department of Mathematics and Statistics, University College of Science, Mohanlal Sukhadia University, Udaipur-313001 Rajasthan (INDIA)
Abstract :

The objective of this paper is to investigate the behaviour of Bianchi Type-VIII Inflationary Cosmological Models with Flat Potential for Stiff Fluid Distribution. To find the solution of thes models we consider that the expansion theta is proportional to the shear sigma, which leads to B = An and potential V (phi ) as a constant. The behaviour of these models from physical and geometrical aspects are also discussed.

Keyword : Bianchi Type-VIII, Inflationary Universe, Stiff Fluid
Paper Download Count : 60
View Count : 66
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