Physics – High Energy Physics – High Energy Physics - Theory
Scientific paper
2004-12-20
Phys.Lett. B610 (2005) 18-22
Physics
High Energy Physics
High Energy Physics - Theory
10 pages
Scientific paper
10.1016/j.physletb.2005.02.006
We discuss the relationship between holographic entropy bounds and gravitating systems. In order to obtain a holographic energy density, we introduce the Bekenstein-Hawking entropy $S_{\rm BH}$ and its corresponding energy $E_{\rm BH}$ using the Friedman equation. We show that the holographic energy bound proposed by Cohen {\it et al} comes from the Bekenstein-Hawking bound for a weakly gravitating system. Also we find that the holographic energy density with the future event horizon deriving an accelerating universe could be given by vacuum fluctuations of the energy density.
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