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Cosmic accelerated expansion and the entropy-corrected holographic dark energy

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Abstract

By considering the logarithmic correction to the energy density, we study the behavior of Hubble parameter in the holographic dark energy model. We assume that the universe is dominated by interacting dark energy and matter and the accelerated expansion of the universe, which may be occurred in the early universe or late time, is studied.

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Authors and Affiliations

  1. Department of Physics, University of Tehran, P.O.B. 14395-547, Tehran, Iran

    H. Mohseni Sadjadi

  2. Center for Advanced Mathematics and Physics, National University of Sciences and Technology, H-12, Islamabad, Pakistan

    Mubasher Jamil

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  1. H. Mohseni Sadjadi
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  2. Mubasher Jamil
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Correspondence to Mubasher Jamil.

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Sadjadi, H.M., Jamil, M. Cosmic accelerated expansion and the entropy-corrected holographic dark energy. Gen Relativ Gravit 43, 1759–1775 (2011). https://doi.org/10.1007/s10714-011-1155-0

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