Quantum dust cores of rotating black holes
Abstract
Abstract Black holes are spacetimes that should describe the end state of the gravitational collapse of huge amounts of quantum matter. A quantum description of dust cores for black hole geometries that accounts for the large number of matter constituents can be obtained by quantising the geodesic motion of dust particles and finding the corresponding many-body ground state. We here generalise previous works in spherical symmetry to rotating geometries and show the effect of angular momentum on the size of the core and effective interior geometry.
Fields of Study & Subjects
Quantum Electrodynamics and Casimir Effect
Astrophysical Phenomena and Observations
Black Holes and Theoretical Physics
Publication details
- Journal / source
- Journal of Cosmology and Astroparticle Physics
- Volume
- 2026
- Issue
- 08
- Pages
- 061–061
- Publication date
- 1 August 2026
- Language
- EN