Kerr Black Hole Dynamics from an Extended Polyakov Action
Abstract
We examine a hypersurface model for the classical dynamics of spinning black holes. Under specific, rigid geometric constraints, it reveals an intriguing solution resembling expectations for the Kerr Black hole three-point amplitude. We explore various generalizations of this formalism and outline potential avenues for applying it to analyze the attraction of spinning black holes.
Fields of Study & Subjects
Black Holes and Theoretical Physics
Noncommutative and Quantum Gravity Theories
Astrophysical Phenomena and Observations
Publication details
- Journal / source
- Physical Review Letters
- Publisher
- American Physical Society (APS)
- Volume
- 136
- Issue
- 7
- Pages
- 071601–071601
- Publication date
- 28 January 2026
- Language
- EN