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Observables for two-dimensional black holes

J. Gegenberg

G. Kunstatter and D. Louis-Martinez

  • Department of Mathematics and Statistics, University of New Brunswick, Fredericton, New Brunswick, Canada E3B 5A3

  • Department of Physics and Winnipeg Institute of Theoretical Physics, University of Winnipeg, Winnipeg, Manitoba, Canada R3B 2E9

Phys. Rev. D 51, 1781 – Published 15 February, 1995

DOI: https://doi.org/10.1103/PhysRevD.51.1781

Abstract

We consider the most general dilaton gravity theory in 1+1 dimensions. By suitably parametrizing the metric and scalar field we find a simple expression that relates the energy of a generic solution to the magnitude of the corresponding Killing vector. In theories that admit black hole solutions, this relationship leads directly to an expression for the entropy S=2πτ0/G, where τ0 is the value of the scalar field (in this parametrization) at the event horizon. This result agrees with the one obtained using the more general method of Wald. Finally, we point out an intriguing connection between the black hole entropy and the imaginary part of the ‘‘phase’’ of the exact Dirac quantum wave functionals for the theory.

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