Semiclassical quantum states for black holes
General Relativity and Quantum Cosmology
2009-10-30 v1
Abstract
I discuss the semiclassical approximation for the Wheeler-DeWitt equation when applied to the CGHS model and spherically symmetric gravity. Special attention is devoted to the issues of Hawking radiation, decoherence of semiclassical states, and black hole entropy.
Cite
@article{arxiv.gr-qc/9701018,
title = {Semiclassical quantum states for black holes},
author = {Claus Kiefer},
journal= {arXiv preprint arXiv:gr-qc/9701018},
year = {2009}
}
Comments
8 pages, LATEX, contribution for the Second Conference on Constrained Dynamics and Quantum Gravity, Santa Margherita, Italy, September 1996