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Geometric Resolution of Schwarzschild Horizon

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arxiv 2303.10186 v1 pith:GMQHHTPM submitted 2023-03-17 hep-th gr-qchep-ph

Ibrahima Bah , Pierre Heidmann This is my paper · ORCID
classification hep-thgr-qchep-ph
keywords schwarzschildblackdimensionsfieldgeometricholehorizonresolution
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We provide the first example of a geometric transition that resolves the Schwarzschild black hole into a smooth microstructure in eleven-dimensional supergravity on a seven-torus. The geometry is indistinguishable from a Schwarzschild black hole dressed with a scalar field in four dimensions, referred to as a Schwarzschild scalarwall. In eleven dimensions, the scalar field arises as moduli of the torus. The resolution occurs at an infinitesimal scale above the horizon, where it transitions to a smooth bubbling spacetime supported by M2-brane flux.

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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. The Special Locus

    hep-th 2025-05 conditional novelty 6.0 of 10

    The special locus is equivalent to vanishing twisted gauge fields in 3D and to the 6D identity B2 = 1/4 B1, which trivializes one anti-self-dual tensor multiplet.

  2. Characterizing geodesic deviations in a Topological Star spacetime: massive, charged, spinning and stringy-like objects

    gr-qc 2025-05 conditional novelty 6.0 of 10

    Nearby geodesics, spinning particles, magnetically charged particles and string probes all deviate from geodesic motion in a topological star, reducing to Schwarzschild plus small alpha-dependent corrections.

  3. Localized Black Holes in AdS$_3$: What Happens Below c/12 Stays Below c/12

    hep-th 2024-12 conditional novelty 6.0 of 10

    Localized black holes in AdS3 x S3 x T4 fill the low-energy spectrum, dominate the microcanonical ensemble below a small positive energy, and appear to have the same entanglement entropy as BTZ black holes.

  4. Black hole mimickers: from theory to observation

    gr-qc 2025-05 unverdicted novelty 2.0 of 10

    A field snapshot from a 2025 Princeton workshop: black hole mimickers remain a viable but unproven alternative to black holes, and upcoming gravitational wave and telescope observations should be able to constrain them.

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