Kerr Black Hole Dynamics from an Extended Polyakov Action
arXiv:2503.20538
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 three-point amplitude. We explore various generalizations of this formalism and outline potential avenues for employing it to analyze spinning black hole attraction.
8 pages, 2 figures, version to be published in PRL