International Journal of Theoretical Physics

, Volume 50, Issue 10, pp 3043-3048

Inflationary Scenario in Bianchi Type I Space-Time

  • Raj BaliAffiliated withDepartment of Mathematics, University of Rajasthan Email author 

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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 ∼T 4, almost vanishes in the course of expansion of universe and total energy-momentum tensor reduces to vacuum stress tensor. This leads to ae Ht 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 I Inflationary scenario