Thermodynamics of interacting entropy-corrected holographic dark energy in a non-flat FRW universe

Details Thermodynamics of interacting entropy-corrected holographic dark energy in a non-flat FRW universe Thermodynamics of interacting entropy-corrected holographic dark energy in a non-flat FRW universe

2010-03-10

arxiv.org/abs/1003.2093v2

Int. J. Mod. Phys. D 19 (2010) 1831-1842

Physics

General Physics

14 pages, no figure, accepted by Int. J. Mod. Phys. D

Scientific paper

10.1142/S0218271810018116

A so-called "entropy-corrected holographic dark energy" (ECHDE), was recently proposed to explain the dark energy-dominated universe with the help of quantum corrections to the entropy-area relation in the setup of loop quantum cosmology. Using this new definition, we investigate its thermodynamical features including entropy and energy conservation. We describe the thermodynamical interpretation of the interaction between ECHDE and dark matter in a non-flat universe. We obtain a relation between the interaction term of the dark components and thermal fluctuation. Our study further generalizes the earlier works [M.R. Setare and E.C. Vagenas, Phys. Lett. B 666 (2008) 111; B. Wang et al., Phys. Lett. B 662 (2008) 1] in this direction.

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