Thermodynamical picture of the interacting holographic dark energy model

Details Thermodynamical picture of the interacting holographic dark energy model Thermodynamical picture of the interacting holographic dark energy model

2009-02-24

arxiv.org/abs/0902.4088v1

Physics

High Energy Physics

High Energy Physics - Theory

10 pages, contribution to the anniversary volume "The Problems of Modern Cosmology", on the occasion of the 50th birthday of P

Scientific paper

In the present paper, 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.

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