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Analyzing exact solutions of the Einstein-Maxwell equations in theKerr-Schild formalism we show that black hole horizon is instable with respectto electromagnetic excitations. Contrary to perturbative smooth harmonicsolutions, the exact solutions for electromagnetic excitations on the Kerrbackground are accompanied by singular beams which have very strong backreaction to metric and break the horizon, forming the holes which allowradiation to escape interior of black-hole. As a result, even the weak vacuumfluctuations break the horizon topologically, covering it by a set offluctuating microholes. We conclude with a series of nontrivial consequences,one of which is that there is no information loss inside of black-hole.

Instability of Black Hole Horizon With Respect to Electromagnetic Excitations