Square-root quantization: application to quantum black holes
General Relativity and Quantum Cosmology
2009-10-30 v1
Abstract
Two different ways of quantizing the relativistic Hamiltonian for radial motion in the field of Coulomb-like potential are compared. The results depend slightly on choice of time. In the case of Lorentzian time a Sommerfeld spectrum is recovered. Application to quantum black holes gives a sqrt{n} mass spectrum with about the same numerical factors.
Cite
@article{arxiv.gr-qc/9701017,
title = {Square-root quantization: application to quantum black holes},
author = {Victor Berezin},
journal= {arXiv preprint arXiv:gr-qc/9701017},
year = {2009}
}
Comments
LaTeX file Talk given on the Second Conference on Constrained Dynamics and Quantum Gravity, Santa Margherita, Ligure, Italy, 17-21 September 1996