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arXiv · gr-qc/0404055

Ln(3) and Black Hole Entropy

Olaf Dreyer
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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.

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Olaf Dreyer. 2004-04-14. Ln(3) and Black Hole Entropy. https://doi.org/10.1142/9789812702340_0075

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