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FRW Bulk Viscous Cosmology in Multi Dimensional Space-Time

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Abstract

The exact solutions of the field equations are obtained by using the gamma law equation of state p=(γ−1)ρ in which the parameter γ depends on scale factor R. The fundamental form of γ(R) is used to analyze a wide range of phases in cosmic history: inflationary phase and radiation-dominated phase. The corresponding physical interpretations of cosmological solutions are also discussed in the framework of (n+2) dimensional space time.

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Authors and Affiliations

  1. Dept. of Mathematics, S.G.B. Amravati University, Amravati, 444602, India

    S. D. Katore, A. Y. Shaikh, D. V. Kapse & S. A. Bhaskar

  2. Department of Mathematics, Dr. B.N. College of Engg. & Tech., Yavatmal, 445001, India

    A. Y. Shaikh

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  1. S. D. Katore
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  2. A. Y. Shaikh
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  3. D. V. Kapse
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  4. S. A. Bhaskar
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Correspondence to S. D. Katore.

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Katore, S.D., Shaikh, A.Y., Kapse, D.V. et al. FRW Bulk Viscous Cosmology in Multi Dimensional Space-Time. Int J Theor Phys 50, 2644–2654 (2011). https://doi.org/10.1007/s10773-011-0760-8

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  • DOI: https://doi.org/10.1007/s10773-011-0760-8

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