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.
Casadio R., Harms B., Leblanc Y. (1998). Statistical mechanics of Kerr-Newman dilaton black holes and the bootstrap condition. PHYSICAL REVIEW D, 57(2), 1309-1312 [10.1103/PhysRevD.57.1309].
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.File in questo prodotto:
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