1992
DOI: 10.1142/s021773239200272x
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Thermodynamics of Two-Dimensional Black Holes

Abstract: We explore the thermodynamics of a general class of two-dimensional dilatonic black holes. A simple prescription is given that allows us to compute the mass, entropy and thermodynamic potentials, with results in agreement with those obtained by other methods, when available.

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Cited by 78 publications
(125 citation statements)
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“…Now, the entropy of the fivedimensional black hole (6) in the extremal limit is S = 2π 2 r 2 1 r 5 /4G 5 . Substituting the corresponding two-dimensional quantities into it, in particular G 5 = 2π 2 r 3 5 G 2 , we again find agreement with the formula (20) derived in [25].…”
supporting
confidence: 82%
See 1 more Smart Citation
“…Now, the entropy of the fivedimensional black hole (6) in the extremal limit is S = 2π 2 r 2 1 r 5 /4G 5 . Substituting the corresponding two-dimensional quantities into it, in particular G 5 = 2π 2 r 3 5 G 2 , we again find agreement with the formula (20) derived in [25].…”
supporting
confidence: 82%
“…But because the Bekenstein-Hawking formula cannot be straightforwardly applied in two dimensions, a different method has to be used to calculate the entropy of these black holes. A thermodynamic approach using boundary terms of the action was adopted in [24,25].…”
mentioning
confidence: 99%
“…In each case first a simple and then a more elaborate derivation will be provided or at least sketched. A comparison with previous results [2,12,13,29,34,35] will be postponed until section 5.…”
Section: Thermodynamical Propertiesmentioning
confidence: 92%
“…Some thermodynamical properties of the 2-d CBH (2.10) were studied semi-classically in [42,7]. The entropy of the CBH is 13…”
Section: Entropy and Reflectionmentioning
confidence: 99%