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Reconstructing f(R) modified gravity from ordinary and entropy-corrected versions of the holographic and new agegraphic dark energy models

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Abstract

Here, we peruse cosmological usage of the most promising candidates of dark energy in the framework of f(R) theory. We reconstruct the different f(R) modified gravity models in the spatially flat FRW universe according to the ordinary and entropy-corrected versions of the holographic and new agegraphic dark energy models, which describe accelerated expansion of the universe. We also obtain the equation of state parameter of the corresponding f(R)-gravity models. We conclude that the holographic and new agegraphic f(R)-gravity models can behave like phantom or quintessence models. Whereas the equation of state parameter of the entropy-corrected models can transit from quintessence state to phantom regime as indicated by recent observations.

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  1. Department of Physics, University of Kurdistan, Pasdaran St., Sanandaj, Iran

    K. Karami

  2. Research Institute for Astronomy & Astrophysics of Maragha (RIAAM), Maragha, Iran

    K. Karami

  3. Department of Physics, University of Kurdistan, Pasdaran St., Sanandaj, Iran

    M. S. Khaledian

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Karami, K., Khaledian, M.S. Reconstructing f(R) modified gravity from ordinary and entropy-corrected versions of the holographic and new agegraphic dark energy models. J. High Energ. Phys. 2011, 86 (2011). https://doi.org/10.1007/JHEP03(2011)086

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