Quasilocal thermodynamics of two-dimensional black holes

Details Quasilocal thermodynamics of two-dimensional black holes Quasilocal thermodynamics of two-dimensional black holes

Dec 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996phrvd..54.7476c&link_type=abstract

Physical Review D (Particles, Fields, Gravitation, and Cosmology), Volume 54, Issue 12, 15 December 1996, pp.7476-7482

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9

Quantum Aspects Of Black Holes, Evaporation, Thermodynamics, Canonical Formalism, Lagrangians, And Variational Principles, Gravity In More Than Four Dimensions, Kaluza-Klein Theory, Unified Field Theories, Alternative Theories Of Gravity, Lower Dimensional Models, Minisuperspace Models

Scientific paper

We present a formalism for analyzing the thermodynamics of two-dimensional black holes in finite-sized systems. The thermodynamic variables are defined on a quasilocal surface and are obtained for a general class of dilaton theories of two-dimensional gravity. We also consider the effects of electromagnetic and Liouville matter fields. We illustrate the formalism by computing the thermodynamic properties of two black hole solutions: one obtained from a string-inspired theory and the other being a black hole in the ``R=T'' theory with a Liouville field.

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