Instability of Black Hole Horizon With Respect to Electromagnetic Excitations

Details Instability of Black Hole Horizon With Respect to Electromagnetic Excitations Instability of Black Hole Horizon With Respect to Electromagnetic Excitations

2009-03-18

arxiv.org/abs/0903.3162v3

Gen.Rel.Grav.41:2281-2286,2009

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

v.3: Final published version, 7pages, 3 figures, Essay, First Award of the Gravity Research Foundation 2009

Scientific paper

10.1007/s10714-009-0851-5

Analyzing exact solutions of the Einstein-Maxwell equations in the Kerr-Schild formalism we show that black hole horizon is instable with respect to electromagnetic excitations. Contrary to perturbative smooth harmonic solutions, the exact solutions for electromagnetic excitations on the Kerr background are accompanied by singular beams which have very strong back reaction to metric and break the horizon, forming the holes which allow radiation to escape interior of black-hole. As a result, even the weak vacuum fluctuations break the horizon topologically, covering it by a set of fluctuating microholes. We conclude with a series of nontrivial consequences, one of which is that there is no information loss inside of black-hole.

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