Black Hole Entropy from Spin One Punctures
General Relativity and Quantum Cosmology
2009-11-10 v1 High Energy Physics - Theory
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 correction with definite coefficient (- 3/2) for large area.
Cite
@article{arxiv.gr-qc/0301128,
title = {Black Hole Entropy from Spin One Punctures},
author = {Romesh K. Kaul and S. Kalyana Rama},
journal= {arXiv preprint arXiv:gr-qc/0301128},
year = {2009}
}
Comments
4 pages. RevTex