paper

A new holographic entropy bound from quantum geometry

arXiv:hep-th/0006211 · doi:10.1103/PhysRevD.63.044019

Abstract

A new entropy bound, tighter than the standard holographic bound due to Bekenstein, is derived for spacetimes with non-rotating 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.

4 pages revtex, no figures; some additions made in text, leading to stronger results; minor changes in the list of references

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