Bianchi Type III inflationary cosmological model in General Relativity
Author & Affiliation:
Raj Bali
CSIR Emeritus Scientist Department of Mathematics, University of Rajasthan, Jaipur-302004 (India)
Laxmi Poonia
Department of Mathematics, ManipalUniversity, Jaipur India
Keyword:
Bianchi III,, inflationary, Cosmological, PACS Nos.: 04.20.-q, 04.20 Jb, 04.20.Dv, 04.20 Ex
Issue Date:
August 2011
Abstract:
| Bianchi Type III inflationary cosmological model for massless scalar field with flat potential is investigated. To get the deterministic model of the universe, we have also assumed that the shear (s) is proportional to expansion (q). This leads to B = Cn where B and C are metric potentials and n is a constant. The inflationary scenario in the model is also discussed. |
Pages:
543-548
ISSN:
2319-8044 (Online) - 2231-346X (Print)
Source:
PDF:
DOI:
jusps-A
Share This:
Copy the following to cite this article:
R. Bali; L. Poonia, "Bianchi Type III inflationary cosmological model in General Relativity", Journal of Ultra Scientist of Physical Sciences, Volume 23, Issue 2, Page Number 543-548, 2019Copy the following to cite this URL:
R. Bali; L. Poonia, "Bianchi Type III inflationary cosmological model in General Relativity", Journal of Ultra Scientist of Physical Sciences, Volume 23, Issue 2, Page Number 543-548, 2019Available from: https://www.ultrascientist.org/paper/1519/
This work is licensed under a Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International License
