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Phantom Appearance of Non-phantom Matter in Anisotropic Cosmological Model

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Abstract

Two cosmological models with non-phantom matter having the same expansion of the universe as phantom cosmologies are constructed in anisotropic Bianchi type-V universe. The exact solutions to the corresponding Einstein field equations have been obtained. The statefinder diagnostic pair i.e. {r,s} parameters have been obtained for disordered radiation i.e. γ=1/3. We have also discussed the well-known astrophysical phenomena, namely the look-back time, luminosity distance and event horizon with redshift.

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Acknowledgements

The authors wish to place on record their sincere thanks to the referee for his valuable comments and suggestions.

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Authors and Affiliations

  1. Department of Applied Mathematics, Institute of Technology, Banaras Hindu University, Varanasi, India

    T. Singh

  2. DST-Centre for Interdisciplinary Mathematical Sciences, Faculty of Science, Banaras Hindu University, Varanasi, India

    R. Chaubey

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  1. T. Singh
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  2. R. Chaubey
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Correspondence to R. Chaubey.

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Singh, T., Chaubey, R. Phantom Appearance of Non-phantom Matter in Anisotropic Cosmological Model. Int J Theor Phys 51, 3495–3507 (2012). https://doi.org/10.1007/s10773-012-1235-2

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  • DOI: https://doi.org/10.1007/s10773-012-1235-2

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