Hamiltonian thermodynamics of charged black holes

A. J. M. Medved and G. Kunstatter
Phys. Rev. D 59, 104005 – Published 29 March 1999
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Abstract

We consider the most general diffeomorphism invariant action in 1+1 spacetime dimensions that contains a metric, dilaton and Abelian gauge field, and has at most second derivatives of the fields. Our action contains a topological term (linear in the Abelian field strength) that has not been considered in previous work. We impose boundary conditions appropriate for a charged black hole confined to a region bounded by a surface of fixed dilaton field and temperature. By making some simplifying assumptions about the quantum theory, the Hamiltonian partition function is obtained. We then use the general formalism to study the partition function for a rotating BTZ black hole confined to a box of fixed radius and temperature.

  • Received 19 November 1998

DOI:https://doi.org/10.1103/PhysRevD.59.104005

©1999 American Physical Society

Authors & Affiliations

A. J. M. Medved*

  • Department of Physics and Winnipeg Institute of Theoretical Physics, University of Manitoba, Winnipeg, Manitoba, Canada R3T 2N2

G. Kunstatter

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

  • *Email address: joey@theory.uwinnipeg.ca
  • Email address: gabor@theory.uwinnipeg.ca

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Vol. 59, Iss. 10 — 15 May 1999

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