Inflationary Scenario in Spatially Homogeneous Bianchi Type IX Space-time with Flat Potential in General Relativity
1CSIR Emeritus Scientist Department of Mathematics, University of Rajasthan, Jaipur-302004 (India)
2Department of Mathematics, ManipalUniversity, Jaipur India
Email of Corresponding Author: balir5@yahoo.co.in
Inflationary scenario in spatially homogeneous Bianchi Type IX space-time is investigated. To get the deterministic result, we have considered the potential V(ø) is constant and the scale factor R ~ eHt where H is Hubble constant. We findthat spatial volume (R3) increases exponentially. Thus inflationary scenario exists in Bianchi Type IX space time. The Higgs field decreases slowly. The expansion () is constant, shear () is zero and deceleration parameter (q) = - 1 which indicate that the model represents de-Sitter universe. The model also gives accelerating phase of the universe
Copy the following to cite this article:
RAJ BALI1 and LAXMI POONIA2, "Inflationary Scenario in Spatially Homogeneous Bianchi Type IX Space-time with Flat Potential in General Relativity", Journal of Ultra Scientist of Physical Sciences, Volume 28, Issue 7, Page Number 361-366, 2016Copy the following to cite this URL:
RAJ BALI1 and LAXMI POONIA2, "Inflationary Scenario in Spatially Homogeneous Bianchi Type IX Space-time with Flat Potential in General Relativity", Journal of Ultra Scientist of Physical Sciences, Volume 28, Issue 7, Page Number 361-366, 2016
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