Kerr Black Hole Dynamics from an Extended Polyakov Action

Fuente: arXiv
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Hauptverfasser: Bjerrum-Bohr, N. Emil J., Chen, Gang, Su, Chenliang, Wang, Tianheng
Format: Preprint
Veröffentlicht: 2025
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author Bjerrum-Bohr, N. Emil J.
Chen, Gang
Su, Chenliang
Wang, Tianheng
author_facet Bjerrum-Bohr, N. Emil J.
Chen, Gang
Su, Chenliang
Wang, Tianheng
contents 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.
format Preprint
id arxiv_https___arxiv_org_abs_2503_20538
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Kerr Black Hole Dynamics from an Extended Polyakov Action
Bjerrum-Bohr, N. Emil J.
Chen, Gang
Su, Chenliang
Wang, Tianheng
High Energy Physics - Theory
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.
title Kerr Black Hole Dynamics from an Extended Polyakov Action
topic High Energy Physics - Theory
url https://arxiv.org/abs/2503.20538