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Singularities in 2D and 3D quantum black holes

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arxiv 2310.06014 v2 pith:FUX27M6W submitted 2023-10-09 hep-th gr-qc

Maciej Kolanowski , Marija Tomašević This is my paper · ORCID
classification hep-thgr-qc
keywords blackholesquantumknownsingularitiessolutionsaccountedarise
verification ladder T0 review T1 audit T2 compute T3 formal
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We study black holes in two and three dimensions that have spacelike curvature singularities behind horizons. The 2D solutions are obtained by dimensionally reducing certain 3D black holes, known as quantum BTZ solutions. Furthermore, we identify the corresponding dilaton potential and show how it can arise from a higher-dimensional theory. Finally, we show that the rotating BTZ black hole develops a singular inner horizon once quantum effects are properly accounted for, thereby solidifying strong cosmic censorship for all known cases.

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Cited by 2 Pith papers

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

  1. Timelike entanglement and central charge for quantum BTZ black holes

    hep-th 2025-07 reject novelty 5.0 of 10

    The paper numerically computes timelike entanglement entropy for quantum BTZ black holes and claims that the effective central charge drops sharply as quantum backreaction crosses a critical value.

  2. Cauchy-horizon flux coefficients in the reduced Polyakov model

    gr-qc 2025-11 reject novelty 4.0 of 10

    The abstract gives the inner-horizon flux coefficient F_-^∞ = t_v - Nκ_-^2/(48π) and its cancellation surface; the supplied full text instead claims a state-independent trace-anomaly enforcement of strong cosmic censo...

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