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Scalar Field Reconstruction of Power-Law Entropy-Corrected HDE

A so called "power-law entropy-corrected holographic dark energy" (PLECHDE) was recently proposed to explain the dark energy dominated universe. This model is based on the power-law corrections to black hole entropy which appear in dealing with the entanglement of quantum fields between inside and outside of the horizon. In this paper, we suggest a correspondence between interacting PLECHDE and tachyon, quintessence, K-essence and dilaton scalar field models of dark energy in a non-flat FRW universe. Then, we reconstruct the potential terms accordingly, and present the dynamical equations which describe the evolution of the scalar field dark energy models.

preprint2011arXivOpen access
Esmaeil EbrahimiAhmad Sheykhi
hep-th
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Esmaeil EbrahimiAhmad Sheykhi

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