Black Hole Entropy from Spin One Punctures

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.

4 pages. RevTex

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• The asymptotic quasinormal mode spectrum of non-rotating black holes
• Dirty black holes: Quasinormal modes
• Quantum Black Holes: Entropy and Entanglement on the Horizon
• Asymptotic quasinormal modes of Reissner-Nordström and Kerr black holes
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• Schwarzschild horizon dynamics and SU(2) Chern-Simons theory
• Intermediate Asymptotics of the Kerr Quasinormal Spectrum
• Topological parameters in gravity
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• Canonical Partition function of Loop Black Holes
• Statistical analysis of entropy correction from topological defects in Loop Black Holes
• Dark Energy From The Gravity Vacuum
• Logarithmic Corrections to the Black Hole Entropy Product of ${\mathcal{H}}^{\pm }$ via Cardy Formula