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Holographic Dark Energy in Brans-Dicke Cosmology with Granda-Oliveros Cut-off

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Abstract

Motivated by the recent works of one of us (Karami and Fehri, Int. J. Theor. Phys. 49:1118, 2010; Phys. Lett. B 684:61, 2010), we study the holographic dark energy in Brans-Dicke gravity with the Granda-Oliveros cut-off proposed recently in literature. We find out that when the present model is combined with Brans-Dicke field the transition from normal state where w D >−1 to the phantom regime where w D <−1 for the equation of state of dark energy can be more easily achieved for than when resort to the Einstein field equations is made. Furthermore, the phantom crossing is more easily achieved when the matter and the holographic dark energy undergo an exotic interaction. We also calculate some relevant cosmological parameters and their evolution.

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Authors and Affiliations

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

    Mubasher Jamil

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

    K. Karami & Z. Azarmi

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

    K. Karami & A. Sheykhi

  4. Department of Physics, Shahid Bahonar University, P.O. Box 76175, Kerman, Iran

    A. Sheykhi & E. Kazemi

Authors
  1. Mubasher Jamil
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  2. K. Karami
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  3. A. Sheykhi
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  4. E. Kazemi
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  5. Z. Azarmi
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Correspondence to Mubasher Jamil.

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Jamil, M., Karami, K., Sheykhi, A. et al. Holographic Dark Energy in Brans-Dicke Cosmology with Granda-Oliveros Cut-off. Int J Theor Phys 51, 604–611 (2012). https://doi.org/10.1007/s10773-011-0940-6

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  • DOI: https://doi.org/10.1007/s10773-011-0940-6

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