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Quantum corrections for (anti)-evaporating black hole

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arxiv hep-th/0007172 v1 pith:ODQT7FY5 submitted 2000-07-21 hep-th

Maja Buric , Voja Radovanovic This is my paper · ORCID
classification hep-th
keywords blackholeanticorrectionsevaporatingmodelquantumspherically
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In this paper we analyse the quantum correction for Schwarzschild black hole in the Unruh state in the framework of spherically symmetric gravity (SSG) model. SSG is a two-dimensional dilaton model which is obtained by spherically symmetric reduction from the four-dimensional theory. We find the one-loop geometry of the (anti)-evaporating black hole and corrections for mass, entropy and apparent horizon.

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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. 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. Quantum Critical Collapse Abhors a Naked Singularity

    gr-qc 2025-09 unverdicted novelty 6.0 of 10

    One-loop quantum vacuum polarization in Einstein-scalar critical collapse generates a horizon and finite mass gap, enforcing black hole formation even under arbitrary fine-tuning.

  3. (Anti-)evaporation of Schwarzschild-de Sitter black holes revisited

    gr-qc 2019-08 conditional novelty 6.0 of 10

    Within the Bousso-Hawking effective action, the Schwarzschild-de Sitter asymptotic is excluded, which undermines earlier anti-evaporation results that used the Nariai limit.

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