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arXiv · 0801.4478

Thermodynamical Interpretation of the Interacting Holographic Dark Energy Model in a non-flat Universe

M. R. Setare·Elias C. Vagenas
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Abstract

Motivated by the recent work of Wang, Lin, Pavon, and Abdalla [1], we generalize their work to the non-flat case. In particular, we provide a thermodynamical interpretation for the holographic dark energy model in a non-flat universe. For this case, the characteristic length is no more the radius of the event horizon (R_E) but the event horizon radius as measured from the sphere of the horizon (L). Furthermore, when interaction between the dark components of the holographic dark energy model in the non-flat universe is present its thermodynamical interpretation changes by a stable thermal fluctuation. A relation between the interaction term of the dark components and this thermal fluctuation is obtained. In the limiting case of a flat universe, i.e. k=0, all results given in [1] are obtained.

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M. R. Setare, Elias C. Vagenas. 2008-07-09. Thermodynamical Interpretation of the Interacting Holographic Dark Energy Model in a non-flat Universe. https://doi.org/10.1016/j.physletb.2008.07.013

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