The Bekenstein-Hawking entropy of a Kerr-Newman dilaton black hole is computed in a perturbative expansion in the charge-to-mass ratio. The most probable configuration for a gas of such black holes is analyzed in the microcanonical formalism and it is argued that it does not satisfy the equipartition principle but does satisfy a bootstrap condition. © 1998 The American Physical Society.

Statistical mechanics of Kerr-Newman dilaton black holes and the bootstrap condition

Casadio R.;
1998

Abstract

The Bekenstein-Hawking entropy of a Kerr-Newman dilaton black hole is computed in a perturbative expansion in the charge-to-mass ratio. The most probable configuration for a gas of such black holes is analyzed in the microcanonical formalism and it is argued that it does not satisfy the equipartition principle but does satisfy a bootstrap condition. © 1998 The American Physical Society.
1998
Casadio R.; Harms B.; Leblanc Y.
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11585/875099
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