A new holographic entropy bound from quantum geometry

Physics – High Energy Physics – High Energy Physics - Theory

Scientific paper

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

Scientific paper

10.1103/PhysRevD.63.044019

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.

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