Geometric Resolution of Schwarzschild Horizon
Ibrahima Bah, Pierre Heidmann

TL;DR
This paper presents a geometric transition in eleven-dimensional supergravity that smooths out the Schwarzschild black hole into a microstructured spacetime supported by M2-brane flux, revealing new microstate geometries.
Contribution
It provides the first explicit example of a geometric resolution of Schwarzschild horizon into a smooth microstructure in higher-dimensional supergravity.
Findings
Resolution occurs at an infinitesimal scale above the horizon.
The smooth microstructure is supported by M2-brane flux.
The geometry matches a Schwarzschild scalarwall in four dimensions.
Abstract
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.
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsBlack Holes and Theoretical Physics · Astrophysical Phenomena and Observations
