Chaotization inside Quantum Black Holes
Andrea Addazi

TL;DR
This paper proposes that quantum black holes can be modeled as a system of horizonless conic singularities, revealing how their horizon geometry and entropy can be reconstructed and how infalling information becomes chaotic, impacting the information paradox.
Contribution
It introduces a novel model of quantum black holes using conic singularities and links it to the Wheeler-De Witt equation, providing insights into horizon structure and information chaos.
Findings
Reconstruction of horizon geometry from conic singularities
Chaotic infall of information within the system
Implications for black hole entropy and information paradox
Abstract
We show how the horizon geometry and entropy of a Semiclassical Black Hole can be reconstructed from a system of horizonless conic singularities with average opening angle at the horizon . This conclusion is strongly motivated by a generalized Wheeler-De Witt equation for quantum black holes. We will argument how infalling information will be inevitably chaotized in these systems. A part of the initial probability density will be trapped inside the system, in back and forth scatterings among conic singularities, for a characteristic time close to the Semiclassical BH life-time. Further implications on information paradoxes are discussed.
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Taxonomy
TopicsCosmology and Gravitation Theories · Quantum Mechanics and Applications · Black Holes and Theoretical Physics
