Generalized Laplace Method for Simple Determination of Kerr-Newman Black Hole Horizon Radius

Details Generalized Laplace Method for Simple Determination of Kerr-Newman Black Hole Horizon Radius Generalized Laplace Method for Simple Determination of Kerr-Newman Black Hole Horizon Radius

2008-11-26

arxiv.org/abs/0811.4297v1

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

4 pages, no figures

Scientific paper

In this work we present a generalized Laplace method for a formal, simple, quasi-classical, determination of the outer and inner horizon radius of Kerr-Newman black hole. We consider classical gravitational interaction between a thin, with homogeneously distributed mass and electric charge, spherical (black) shell and a probe particle. Also, we use relativistic equivalence principle. Finally we suppose that probe particle propagates radially to shell with speed of light while tangentially it rotates in common with shell, so that total energy of a probe particle equals zero.

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