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Universe Described by Kaluza–Klein Space Time with Viscous Modified Cosmic Chaplygin Gas in General Relativity

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Abstract

In this paper, we constructed Kaluza–Klein FRW model with modified cosmic Chaplygin gas in presence of bulk viscosity. We used exponential function method (Ganji and Hasheni Kachapi 2011) to solve non-linear differential equation and obtained time dependent dark energy density. We explained the nature of the energy density for different values of parameters through graphical representation briefly. Also, we investigated the nature of the energy density with and without bulk viscosity. Finally we discussed stability of this theory and obtained that, the model does not have any singularity in presence and absence of bulk viscosity.

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Acknowledgments

The authors would like to thank the anonymous referee for his valuable suggestions.

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Authors and Affiliations

  1. Department of Mathematics, BITS-Pilani, K K Birla Goa Campus, Goa, 403726, India

    G. C. Samanta

  2. Department of Mathematics, Visvesvaraya National Institute of Technology, Nagpur, 440010, India

    Binaya K. Bishi

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  1. G. C. Samanta
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  2. Binaya K. Bishi
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Correspondence to G. C. Samanta.

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Samanta, G.C., Bishi, B.K. Universe Described by Kaluza–Klein Space Time with Viscous Modified Cosmic Chaplygin Gas in General Relativity. Iran J Sci Technol Trans Sci 40, 245–254 (2016). https://doi.org/10.1007/s40995-016-0089-5

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