Hologrphy and holographic dark energy model
arXiv:hep-th/0505175 · doi:10.1088/0264-9381/22/22/014
Abstract
The holographic principle is used to discuss the holographic dark energy model. We find that the Bekenstein-Hawking entropy bound is far from saturation under certain conditions. A more general constraint on the parameter of the holographic dark energy model is also derived.
no figures, use revtex, v2: use iop style, some typos corrected and references updated, will appear in CQG
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