Causality bounds chaos in geodesic motions

Abstract

Predictability is ensured by causality while lost in chaos. To reconcile these two popular notions, we study chaos in geodesic motions in generic curved spacetimes with external potentials, where causality is controlled by a scalar potential. We develop a reparametrization-independent method to analytically estimate the Lyapunov exponent $\lambda$ of a particle motion. We show that causality gives the universal upper bound $\lambda \propto E(E\to \infty )$, which coincides with the chaos energy bound proposed by Murata, Tanahashi, Watanabe, and one of the authors (K.H.). We also find that the chaos bound discovered by Maldacena, Shenker, and Stanford can be violated in particular potentials, even with causality. Our estimates, although waiting for numerical confirmation, reveal the hidden nature of physical theories: causality bounds chaos.

arXiv comment20 pages. v2: typos corrected, references added

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• Bounds for Lyapunov exponent of circular light orbits in black holes
• Stationary equilibrium of test particles near charged black branes with the hyperscaling violating factor
• Motions of spinning particles and chaos bound in Reissner-Nordström spacetime
• Adiabatic Gauge Potential as a Tool for Detecting Chaos in Classical Systems