Holographic principle in the BDL brane cosmology

preprint2001arXivOpen access

Abstract

We study the holographic principle in the brane cosmology. Especially we describe how to accommodate the 5D anti de Sitter Schwarzschild (AdSS5_5) black hole in the Binetruy-Deffayet-Langlois (BDL) approach of brane cosmology. It is easy to make a connection between a mass MM of the AdSS5_5 black hole and a conformal field theory (CFT)-radiation dominated universe on the brane in the moving domain wall approach. But this is not established in the BDL approach. In this case we use two parameters C1,C2C_1, C_2 in the Friedmann equation. These arise from integration and are really related to the choice of initial bulk matter. If one chooses a bulk energy density ρBρ_B to account for a mass MM of the AdSS5_5 black hole and the static fifth dimension, a CFT-radiation term with ρCFT∼M/a4ρ_{CFT} \sim M/a^{4} comes out from the bulk matter without introducing a localized matter distribution on the brane. This means that the holographic principle can be established in the BDL brane cosmology.

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