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A Non-Singular Black Hole

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arxiv gr-qc/9804070 v1 pith:GUR7VT2B submitted 1998-04-26 gr-qc

Aleksandar Bogojevic (Institute of Physics , Belgrade) , Dejan Stojkovic (Case Western Reserve University) This is my paper · ORCID
classification gr-qc
keywords blackcghsholesolutionasymptoticalycompletelydeformationdilaton
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We present a completely integrable deformation of the CGHS dilaton gravity model in two dimensions. The solution is a singularity free black hole that at large distances asymptoticaly joins to the CGHS solution.

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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. Resolving Black Hole Singularities in Jackiw-Teitelboim Gravity

    hep-th 2026-02 conditional novelty 6.0 of 10

    In JT gravity, the left confining potential required by spectral discreteness makes the wormhole length turn around and plateau, allowing boundary time to run past the would-be singularity and eliminating future horizons.

  2. The fate of Schwarzschild--de Sitter black holes: nonequilibrium evaporation

    hep-th 2025-11 conditional novelty 5.0 of 10

    In the Unruh–de Sitter state the anomaly flux J=(N/48π)(κ_b²−κ_c²) is positive throughout the static patch, so every neutral SdS black hole evaporates monotonically and only the Nariai limit has zero flux.

  3. Observing the eye of the storm I: testing regular black holes with LVK and EHT observations

    gr-qc 2024-11 conditional novelty 5.0 of 10

    EHT shadow sizes and LIGO/Virgo/KAGRA inspiral waveforms allow only small values of the dimensionless regularity parameter ℓ in the Ghosh-Simpson-Visser regular black hole.

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