We show how the horizon geometry and entropy of a Semiclassical Black Hole canbe reconstructed from a system of N 1 horizonless conic singularities with average openingangle at the horizon Θ = 2π. This conclusion is strongly motivated by a generalized WheelerDe Witt equation for quantum black holes. We will argument how infalling information will beinevitably chaotized in these systems. A part of the initial probability density will be trappedinside the system, in back and forth scatterings among conic singularities, for a characteristictime close to the Semiclassical BH life-time. Further implications on information paradoxes arediscussed.
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