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

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

1997-06-02

arxiv.org/abs/gr-qc/9706005v1

Phys.Rev. D57 (1998) 1309-1312

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

RevTeX, 5 pages, 2 PS figures included (requires epsf), submitted to Phys. Rev. Lett

Scientific paper

10.1103/PhysRevD.57.1309

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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