Bianchi Type V Barotropic Perfect Fluid Cosmological Model in Lyra Geometry

Details Bianchi Type V Barotropic Perfect Fluid Cosmological Model in Lyra Geometry Bianchi Type V Barotropic Perfect Fluid Cosmological Model in Lyra Geometry

May 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009ijtp...48.1523b&link_type=abstract

International Journal of Theoretical Physics, Volume 48, Issue 5, pp.1523-1533

Physics

5

Bianchi V, Barotropic, Lyra

Scientific paper

We have investigated Bianchi Type V barotropic perfect fluid cosmological model in Lyra geometry. To get the deterministic model of the universe, we have assumed the barotropic perfect fluid condition p= γ ρ, 0≤ γ≤1 and energy conservation equation i.e. T {/i; j j }=0. The physical and geometrical aspects of the model are discussed. The special cases for γ=1 (stiff fluid distribution), γ=0 (dust distribution), γ=1/3 (disordered radiation) are also discussed.

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