In the moving mirror analog of black hole evaporation, restoring information by vacuum entanglement requires emitting at least as many late-time inertial particles as Hawking particles, and for real black holes this is energetically impossible.
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The Particle and Energy Cost of Entanglement of Hawking Radiation with the Final Vacuum State
In the moving mirror analog of black hole evaporation, restoring information by vacuum entanglement requires emitting at least as many late-time inertial particles as Hawking particles, and for real black holes this is energetically impossible.