International Journal of Theoretical Physics

, 50:3043

Inflationary Scenario in Bianchi Type I Space-Time


DOI: 10.1007/s10773-011-0804-0

Cite this article as:
Bali, R. Int J Theor Phys (2011) 50: 3043. doi:10.1007/s10773-011-0804-0


Inflationary scenario in Bianchi Type I space-time is discussed. To get the deterministic model of the universe, it has been considered that the energy-momentum tensor of particles ∼T4, almost vanishes in the course of expansion of universe and total energy-momentum tensor reduces to vacuum stress tensor. This leads to aeHt where a is scale factor and H the Hubble constant and effective potential V(φ)=constant where φ is Higg’s field and n is a constant. The physical and geometrical aspects of the model in the context of inflationary scenario are also discussed.


Bianchi IInflationary scenario

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© Springer Science+Business Media, LLC 2011

Authors and Affiliations

  1. 1.Department of MathematicsUniversity of RajasthanJaipurIndia