Astrophysical black holes (BHs) are universally expected to be described by the Kerr metric, a stationary, vacuum solution of general relativity (GR). Indeed, by imaging M87* and Sgr A …
E Gallo, T Mädler - arXiv preprint arXiv:2412.10328, 2024 - arxiv.org
Chaotic systems near black holes satisfy a universal bound, $\lambda\leq\kappa_H $ linking the Lyapunov coefficient $\lambda $ associated with unstable orbits to surface gravity …