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

R. Casadio·B. Harms·Y. Leblanc
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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 a bootstrap condition. It is also suggested that the present results are further support for an interpretation of black holes as excitations of extended objects.

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R. Casadio, B. Harms, Y. Leblanc. 1997-06-02. Statistical mechanics of Kerr-Newman dilaton black holes and the bootstrap condition. https://doi.org/10.1103/physrevd.57.1309

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