Entropy using Path Integrals for Quantum Black Hole Models

Details Entropy using Path Integrals for Quantum Black Hole Models Entropy using Path Integrals for Quantum Black Hole Models

2000-03-08

arxiv.org/abs/gr-qc/0003023v2

Gen.Rel.Grav.33:913-919,2001

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

7 pages, LaTeX, no figures

Scientific paper

10.1023/A:1010216126590

Several eigenvalue equations that could describe quantum black holes have been proposed in the canonical quantum gravity approach. In this paper, we choose one of the simplest of these quantum equations to show how the usual Feynman's path integral method can be applied to obtain the corresponding statistical properties. We get a logarithmic correction to the Bekenstein-Hawking entropy as already obtained by other authors by other means.

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