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The End of a Black Hole's Evaporation -- Part II

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arxiv 2105.06876 v2 pith:S4MGCJHL submitted 2021-05-14 gr-qc

Farshid Soltani , Carlo Rovelli , Pierre Martin-Dussaud This is my paper · ORCID
classification gr-qc
keywords blackevaporationholeamplitudecovariantderiveexplicitexpression
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We derive an explicit expression for the transition amplitude from black to white hole horizon at the end of Hawking evaporation using covariant loop quantum gravity.

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Cited by 3 Pith papers

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

  1. Studying replica wormholes and the Page curve with simplicial quantum gravity

    hep-th 2025-04 conditional novelty 6.0 of 10

    A coarse simplicial quantum gravity model produces semiclassical saddles whose swap entropy rises and then falls, reproducing the Page transition at n→1+.

  2. Quantum Schwarzschild-(A)dS Black Holes: Unitarity and Singularity Resolution

    hep-th 2025-02 conditional novelty 6.0 of 10

    Unitarity in unimodular time self-adjointness resolves the Schwarzschild-(A)dS singularity and yields a quantum-corrected metric interpolating between black and white hole states.

  3. The Case For Black Hole Remnants: A Review

    gr-qc 2024-11 unverdicted novelty 2.0 of 10

    A review arguing that black hole remnants remain viable and that the species and entropy objections to them are not decisive, so remnants could resolve the information paradox.

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