A new holographic entropy bound from quantum geometry
High Energy Physics - Theory
2009-10-31 v2 General Relativity and Quantum Cosmology
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.
Cite
@article{arxiv.hep-th/0006211,
title = {A new holographic entropy bound from quantum geometry},
author = {Saurya Das and Romesh K Kaul and Parthasarathi Majumdar},
journal= {arXiv preprint arXiv:hep-th/0006211},
year = {2009}
}
Comments
4 pages revtex, no figures; some additions made in text, leading to stronger results; minor changes in the list of references