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A Self-consistent Model of the Black Hole Evaporation

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arxiv 1302.4733 v1 pith:J2KJ6AN7 submitted 2013-02-19 hep-th

Hikaru Kawai , Yoshinori Matsuo , Yuki Yokokura This is my paper · ORCID
classification hep-th
keywords blackevaporationholehorizonmodelnullself-consistentsingularity
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We construct a self-consistent model which describes a black hole from formation to evaporation including the back reaction from the Hawking radiation. In the case where a null shell collapses, at the beginning the evaporation occurs, but it stops eventually, and a horizon and singularity appear. On the other hand, in the generic collapse process of a continuously distributed null matter, the black hole evaporates completely without forming a macroscopically large horizon nor singularity. We also find a stationary solution in the heat bath, which can be regarded as a normal thermodynamic object.

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Cited by 4 Pith papers

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

  1. Unveiling horizons in quantum critical collapse

    gr-qc 2025-09 unverdicted novelty 7.0 of 10

    Semiclassical quantum corrections in critical collapse yield a finite mass gap and transition from classical Type II to quantum Type I behavior, providing a quantum enforcement of weak cosmic censorship.

  2. Black Mirrors: CPT-Symmetric Alternatives to Black Holes

    hep-th 2024-12 reject novelty 5.0 of 10

    A two-sheeted spacetime glued at the black hole horizon, called the black mirror, is proposed as a singularity-free, CPT-symmetric alternative to black holes.

  3. Characterizing the Properties and Constitution of Compact Objects in Gravitational-Wave Binaries

    gr-qc 2024-11 conditional novelty 5.0 of 10

    Tidal heating imprints from black hole horizons can be captured by two effective parameters and modeled through merger, offering a future test to distinguish black holes from exotic horizonless objects.

  4. UV Effects and Short-Lived Hawking Radiation: Alternative Resolution of Information Paradox

    hep-th 2024-11 unverdicted novelty 5.0 of 10

    Hawking radiation terminates around the scrambling time due to trans-Planckian stringy effects in GUP and string-field-theory-inspired toy models, yielding negligible evaporation and a mostly classical black hole.

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