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Ln(3) and Black Hole Entropy
We review an idea that uses details of the quasinormal mode spectrum of a
black hole to obtain the Bekenstein-Hawking entropy of in Loop Quantum
Gravity. We further comment on a recent proposal concerning the quasinormal
mode spectrum of rotating black holes. We conclude by remarking on a recent
proposal to include supersymmetry.Comment: Contribution to the Proceedings of the 3rd International Symposium on
Quantum Theory and Symmetries, Cincinnati, September 2003, added references
to the numerical investigations of Kerr quasinormal modes by Berti et. a
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