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About the Incompleteness of the Semiclassical Picture in the BH-Information Paradox and the Quantum Hair emerging from the Coupling of Quantum Matter and Quantum Space-Time Degrees of Freedom

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arxiv 1503.07312 v2 pith:J5JMJAP7 submitted 2015-03-25 gr-qc hep-th

classification gr-qchep-th
keywords quantumstatefinalblackdegreesevaporationfreedomhair
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We argue that the semiclassical analysis of the black hole information paradox is incomplete and has to be completed by an explicit entanglement of matter and quantum gravity degrees of freedom. We study in detail the evaporation process from beginning to end in the light of our extension and show that a pure initial state remains pure over the full evaporation process, including the final state which remains after the black hole has completely evaporated. By the same token we show how the quantum hair is encoded in the micro structure of the (final) gravitational state which is entangled with the (final) radiation state.

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Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. The Black Hole Singularity as a Thermodynamic System being the Seat of BH Entropy

    gr-qc 2024-11 reject novelty 4.0 of 10

    The paper proposes that the black hole singularity, modeled as a random network of elementary degrees of freedom, carries entropy proportional to M^2, matching the scaling of Bekenstein-Hawking entropy.

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