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Bianchi Type V Barotropic Perfect Fluid Cosmological Model in Lyra Geometry

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Abstract

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 j i;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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Authors and Affiliations

  1. Department of Mathematics, University of Rajasthan, Jaipur, 302004, India

    Raj Bali

  2. Department of Mathematics, Jaipur Engineering College, Jaipur, 303101, India

    Naresh K. Chandnani

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  1. Raj Bali
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  2. Naresh K. Chandnani
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Correspondence to Raj Bali.

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Bali, R., Chandnani, N.K. Bianchi Type V Barotropic Perfect Fluid Cosmological Model in Lyra Geometry. Int J Theor Phys 48, 1523–1533 (2009). https://doi.org/10.1007/s10773-009-0002-5

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  • DOI: https://doi.org/10.1007/s10773-009-0002-5

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