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arxiv: 1105.1008 · v2 · pith:ROKMJXYXnew · submitted 2011-05-05 · 🌀 gr-qc · astro-ph.CO· hep-th

Interacting viscous entropy-corrected holographic scalar field models of dark energy with time-varying G in modified FRW cosmology

classification 🌀 gr-qc astro-ph.COhep-th
keywords interactingviscousdarkechdeentropy-correctedmodelcosmologyenergy
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We study the entropy-corrected version of the holographic dark energy (HDE) model in the framework of modified FRW cosmology. We consider a non-flat universe filled with an interacting viscous entropy-corrected HDE (ECHDE) with dark matter. We also include the case of variable gravitational constant G in our model. We obtain the equation of state and the deceleration parameters of the interacting viscous ECHDE. Moreover, we reconstruct the potential and the dynamics of the quintessence, tachyon, K-essence and dilaton scalar field models according to the evolutionary behavior of the interacting viscous ECHDE model with time-varying G.

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