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. |
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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/