Black Holes as Rubik's Cubes
Bart{\l}omiej Czech, Klaus Larjo, Moshe Rozali

TL;DR
This paper introduces a simplified quantum model of black hole evaporation where entanglement diminishes over time, offering insights into how information might escape from black holes.
Contribution
It presents a novel toy model that captures key features of black hole evaporation, including information release and a vacuum state representing complete evaporation.
Findings
Entanglement between interior and exterior diminishes at late times.
The model exhibits the information-free property.
A vacuum state exists for the fully evaporated black hole.
Abstract
We propose a unitary toy model of black hole evaporation, in which the entanglement between the interior and exterior degrees of freedom vanishes at late times. Our model possesses the information-free property and satisfies the niceness conditions discussed in the literature. A key feature of the model is that the Hilbert space of black hole internal states contains a vacuum state corresponding to the completely evaporated black hole, which can be reached from any initial state via the Hawking process. Our model suggests a novel quantum cosmological way in which information can get out of an evaporating black hole.
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