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Stability analysis of a holographic dark energy model

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Abstract

The stability of interacting holographic dark energy model is discussed. It is found that for some class of the rate of interaction between dark matter and dark energy, the system has a natural solution where the universe had been decelerating in the beginning but finally settles down to an accelerated phase of expansion.

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Acknowledgments

N.R. wishes to thank CSIR (India) for financial support.

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Authors and Affiliations

  1. Department of Physical Sciences, Indian Institute of Science Education and Research Kolkata, Mohanpur, 741246, India

    Narayan Banerjee & Nandan Roy

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  1. Narayan Banerjee
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  2. Nandan Roy
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Correspondence to Narayan Banerjee.

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Banerjee, N., Roy, N. Stability analysis of a holographic dark energy model. Gen Relativ Gravit 47, 92 (2015). https://doi.org/10.1007/s10714-015-1933-1

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  • DOI: https://doi.org/10.1007/s10714-015-1933-1

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