On Black Hole Horizon Fluctuations

Details On Black Hole Horizon Fluctuations On Black Hole Horizon Fluctuations

1998-07-23

arxiv.org/abs/gr-qc/9807065v2

Nucl.Phys. B553 (1999) 333-352

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

20 pages; LaTeX2e; to be published in the Nuclear Physics B; Section 3 was revised and Appendix added

Scientific paper

10.1016/S0550-3213(99)00238-2

A study of the high angular momentum particles 'atmosphere' near the Schwarzschild black hole horizon suggested that strong gravitational interactions occur at invariant distance of the order of $\sqrt[3]{M}$ (A. Casher et. al). We present a generalization of this result to the Kerr-Newman black hole case. It is shown that the larger charge and angular momentum black hole bears, the larger invariant distance at which strong gravitational interactions occur becomes. This invariant distance is of order $\sqrt[3]{r_+^2/\hh}.$ This implies, that the Planckian structure of the Hawking radiation of extreme black holes is completely broken.

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