Black Hole Information as Topological Qubits
Erik Verlinde, Herman Verlinde
TL;DR
The paper reframes black hole information as topological qubits arising from non-local, balanced holography between the interior $H$ and entangled environment $E$, with a holographic dictionary linking hidden microscopic data to bulk observables. It introduces Majorana-based topological qubits consisting of a logical (real) qubit and a fixed virtual qubit, and shows how entanglement swapping transfers information from the black hole to Hawking radiation while preserving horizon smoothness. Time evolution is shown to align with Page dynamics, and interior bulk observables can be reconstructed via quantum error correction with controllable accuracy. The approach resolves the firewall/AMPS paradox by separating the carrying of black hole information from the local near-horizon vacuum structure and demonstrates horizon smoothness across black hole ages.
Abstract
The principle of balanced holography, introduced in [1], posits that black hole information is stored in non-local correlations between the interior and exterior. Based on this concept, we propose that black hole information decomposes into elementary units in the form of topological qubits, and is protected from local sources of decoherence. The topological protection mechanism ensures that the horizon of an evaporating black hole stays young and smooth.
