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Black Hole Entropy from Spin One Punctures

Romesh K. Kaul·S. Kalyana Rama
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Abstract

Recent suggestion, that the emission of a quantum of energy corresponding to the asymptotic value of quasinormal modes of a Schwarzschild black hole should be associated with the loss of spin one punctures from the black hole horizon, fixes the Immirzi parameter to a definite value. We show that saturating the horizon with spin one punctures reproduces the earlier formula for the black hole entropy, including the $ln (area)$ correction with definite coefficient (- 3/2) for large area.

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Romesh K. Kaul, S. Kalyana Rama. 2003-01-31. Black Hole Entropy from Spin One Punctures. https://doi.org/10.1103/physrevd.68.024001

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