Causality bounds chaos in geodesic motions
Koji Hashimoto, Kakeru Sugiura

TL;DR
This paper investigates how causality constrains chaos in geodesic motions within curved spacetimes, establishing universal bounds on Lyapunov exponents and exploring conditions under which these bounds can be violated.
Contribution
The authors develop a reparametrization-independent analytical method to estimate Lyapunov exponents and demonstrate causality's role in bounding chaos in particle dynamics.
Findings
Causality imposes a universal upper bound on Lyapunov exponents proportional to energy.
The chaos energy bound aligns with previous theoretical proposals.
Violations of the Maldacena-Shenker-Stanford chaos bound are possible in certain potentials.
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 of a particle motion. We show that causality gives the universal upper bound , 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.
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Taxonomy
TopicsBlack Holes and Theoretical Physics · Geometric Analysis and Curvature Flows · Cosmology and Gravitation Theories
