New holographic entropy bound from quantum geometry
- 29 January 2001
- journal article
- research article
- Published by American Physical Society (APS) in Physical Review D
- Vol. 63 (4) , 044019
- https://doi.org/10.1103/physrevd.63.044019
Abstract
A new entropy bound, tighter than the standard holographic bound due to Bekenstein, is derived for space-times with nonrotating isolated horizons from the quantum geometry approach, in which the horizon is described by the boundary degrees of freedom of a three dimensional Chern-Simons theory.Keywords
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This publication has 14 references indexed in Scilit:
- Logarithmic Correction to the Bekenstein-Hawking EntropyPhysical Review Letters, 2000
- Holographic bound from second law of thermodynamicsPhysics Letters B, 2000
- The holographic principle for general backgroundsClassical and Quantum Gravity, 2000
- Quantum black hole entropyPhysics Letters B, 1998
- Quantum Geometry and Black Hole EntropyPhysical Review Letters, 1998
- From Euclidean to Lorentzian general relativity: The real wayPhysical Review D, 1996
- Linking topological quantum field theory and nonperturbative quantum gravityJournal of Mathematical Physics, 1995
- The world as a hologramJournal of Mathematical Physics, 1995
- Generalized second law of thermodynamics in black-hole physicsPhysical Review D, 1974
- Black Holes and EntropyPhysical Review D, 1973