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Interacting Holographic Polytropic Gas Model of Dark Energy

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Abstract

In this work, we establish a correspondence between the holographic dark energy model and polytropic gas model of dark energy in the FRW universe. This correspondence allows us to reconstruct the potential and the dynamics for the scalar field of the polytropic model according to the evolution of holographic dark energy in the FRW universe.

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Acknowledgements

This work has been supported financially by Research Institute for Astronomy & Astrophysics of Maragha (RIAAM) under research project 1/2782-50.

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Authors and Affiliations

  1. Department of Physics, Faculty of Science, Bu-Ali Sina University, Hamedan, 65178, Iran

    M. Taji & M. Malekjani

  2. Research Institute for Astronomy & Astrophysics of Maragha (RIAAM), P.O. Box 55134-441, Maragha, Iran

    M. Malekjani

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  1. M. Taji
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  2. M. Malekjani
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Correspondence to M. Malekjani.

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Taji, M., Malekjani, M. Interacting Holographic Polytropic Gas Model of Dark Energy. Int J Theor Phys 52, 3405–3412 (2013). https://doi.org/10.1007/s10773-013-1641-0

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  • DOI: https://doi.org/10.1007/s10773-013-1641-0

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