Classical and Quantum Properties of Liouville Black Holes

Preprint

25 April 1994

preprint
Published by arXiv in arXiv

https://doi.org/10.48550/arXiv.gr-qc/9404045

Abstract

Black hole spacetimes can arise when a Liouville field is coupled to two- dimensional gravity. Exact solutions are obtained both classically and when quantum corrections due to back reaction effects are included. The black hole temperature depends upon the mass and the thermodynamic limit breaks down before evaporation of the black hole is complete, indicating that higher-loop effects must be included for a full description of the process.

Keywords

QUANTUM PROPERTIES
LIOUVILLE BLACK
HOLE SPACETIMES
EVAPORATION
SPACETIMES
BLACK HOLE
GRAVITY

All Related Versions

Version 1, 1994-04-25, ArXiv

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