Kerr Black Hole Dynamics from an Extended Polyakov Action
High Energy Physics - Theory
2026-02-13 v2
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.
Cite
@article{arxiv.2503.20538,
title = {Kerr Black Hole Dynamics from an Extended Polyakov Action},
author = {N. Emil J. Bjerrum-Bohr and Gang Chen and Chenliang Su and Tianheng Wang},
journal= {arXiv preprint arXiv:2503.20538},
year = {2026}
}
Comments
8 pages, 2 figures, version to be published in PRL