The Cardy-Verlinde Formula and Topological AdS-Schwarzschild Black Holes
arXiv:hep-th/0105093 · doi:10.1016/S0370-2693(01)00845-0
Abstract
We consider the brane universe in the background of the topological AdS-Schwarzschild black holes. The induced geometry of the brane is that of a flat or an open radiation dominated FRW-universe. Just like the case of a closed radiation dominated FRW-universe, the temperature and entropy are simply expressed in terms of the Hubble parameter and its time derivative when the brane crosses the black hole horizon. We propose the modified Cardy-Verlinde formula which is valid for any values of the curvature parameter k in the Friedmann equations.
9 pages, LaTeX, reference added
References in corpus (3)
Cited by in corpus (19)
- Entropy and universality of Cardy-Verlinde formula in dark energy universe
- Anti-de Sitter Black Holes, Thermal Phase Transition and Holography in Higher Curvature Gravity
- Cosmological and black hole brane-world Universes in higher derivative gravity
- Cardy-Verlinde Formula and Asymptotically de Sitter Spaces
- Quest for Localized 4-D Black Holes in Brane Worlds
- On the Cardy-Verlinde Entropy Formula in Viscous Cosmology
- Holographic principle and dark energy
- Constant Curvature Black Hole and Dual Field Theory
- de Sitter thermodynamics and the braneworld
- A Note on the Cardy-Verlinde Formula
- Entropy Bounds in Geometries
- A plausible upper limit on the number of e-foldings
- Cardy-Verlinde Formula and entropy bounds in Kerr-Newman-AdS/dS black holes backgrounds
- Schwarzschild Black Branes and Strings in higher-dimensional Brane Worlds
- Holographic complexity growth in a FLRW universe
- Brane World in a Topological Black Hole Bulk
- dS/CFT Duality on the Brane with a Topological Twist
- A not so brief commentary on cosmological entropy bounds
- Brane universe and holography in spacetime of charged AdS dilaton black hole