Bekenstein Bound, Holography and Brane Cosmology in Charged Black Hole Backgrounds

Details Bekenstein Bound, Holography and Brane Cosmology in Charged Black Hole Backgrounds Bekenstein Bound, Holography and Brane Cosmology in Charged Black Hole Backgrounds

2001-05-08

arxiv.org/abs/hep-th/0105070v2

Class.Quant.Grav. 18 (2001) 5429-5440

Physics

High Energy Physics

High Energy Physics - Theory

Latex, 17 pages, v2: minor changes, a reference added

Scientific paper

10.1088/0264-9381/18/24/308

We obtain a Bekenstein entropy bound for the charged objects in arbitrary dimensions ($D\ge 4$) using the D-bound recently proposed by Bousso. With the help of thermodynamics of CFTs corresponding to AdS Reissner-Norstr\"om (RN) black holes, we discuss the relation between the Bekenstein and Bekenstein-Verlinde bounds. In particular we propose a Bekenstein-Verlinde-like bound for the charged systems. In the Einstein-Maxwell theory with a negative cosmological constant, we discuss the brane cosmology with positive tension using the Binetruy-Deffayet-Langlois approach. The resulting Friedman-Robertson-Walker equation can be identified with the one obtained by the moving domain wall approach in the AdS RN black hole background. Finally we also address the holographic property of the brane universe.

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