LN(3) and Black Hole Entropy
Abstract
We review an idea that uses details of the quasinormal mode spectrum of a black hole to obtain the Bekenstein-Hawking entropy of A/4 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.
- Publication:
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Quantum Theory and Symmetries
- Pub Date:
- October 2004
- DOI:
- arXiv:
- arXiv:gr-qc/0404055
- Bibcode:
- 2004qts..conf..635D
- Keywords:
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- General Relativity and Quantum Cosmology
- E-Print:
- 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. al