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The Cardy-Verlinde Formula and Asymptotically de Sitter Brane Universe

Donam Youm

hep-tharXiv:hep-th/0111276

Abstract

We consider the brane universe in the bulk background of the topological AdS-Schwarzschild black holes, where the brane tension takes larger value than the fine-tunned value. The resulting universe is radiation dominated and has positive cosmological constant. We obtain the associated cosmological Cardy formula and the Cardy-Verlinde formula. We also derive the Hubble and the Bekenstein entropy bounds from the conjectured holography bound on the Casimir entropy.

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