A self-consistent angular momentum constraint in black hole spacetimes shows MSS chaos bound violations in charged Kiselev black holes are often parameter artifacts while higher-curvature geometries exhibit genuine violations at large charge-to-mass ratios.
Within this framework, the radii of circular orbits are obtained from the equilibrium condition (23)
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Physical constraints on the Maldacena-Shenker-Stanford chaos-bound in black hole spacetimes
A self-consistent angular momentum constraint in black hole spacetimes shows MSS chaos bound violations in charged Kiselev black holes are often parameter artifacts while higher-curvature geometries exhibit genuine violations at large charge-to-mass ratios.