Bianchi Type-VIII Inflationary Cosmological Models with Flat Potential and Stiff perfect Fluid Distribution in General Relativity
Author & Affiliation:
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)
Keyword:
Bianchi Type-VIII, Inflationary Universe, Stiff Fluid
Issue Date:
Nov 2023
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 is proportional to the shear
, which leads to B = An and potential V (
) as a constant. The behaviour of these models from physical and geometrical aspects are also discussed.
Pages:
68-78
ISSN:
2319-8044 (Online) - 2231-346X (Print)
Source:
DOI:
http://dx.doi.org/10.22147/jusps-A/350701
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Copy the following to cite this article:
D. Chhajed; Monika; A. Tyagi, "Bianchi Type-VIII Inflationary Cosmological Models with Flat Potential and Stiff perfect Fluid Distribution in General Relativity", Journal of Ultra Scientist of Physical Sciences, Volume 35, Issue 7, Page Number 68-78, 2023Copy the following to cite this URL:
D. Chhajed; Monika; A. Tyagi, "Bianchi Type-VIII Inflationary Cosmological Models with Flat Potential and Stiff perfect Fluid Distribution in General Relativity", Journal of Ultra Scientist of Physical Sciences, Volume 35, Issue 7, Page Number 68-78, 2023Available from: https://www.ultrascientist.org/paper/1584/
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