Quantum chaos inside Black Holes

We show how semiclassical black holes can be reinterpreted as an effective geometry, composed of a large ensemble of horizonless naked singularities (eventually smoothed at the Planck scale). We call these new items frizzy-balls, which can be rigorously defined by Euclidean path integral approach. This leads to interesting implications about information paradoxes. We demonstrate that infalling information will chaotically propagate inside this system before going to the full quantum gravity regime (Planck scale).

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More references added, few typos corrected

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Quantum black hole
quantum chaos
naked singularities
scale: Planck
black hole: semiclassical
information theory

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