Classical billiards can compute

📅 2025-12-22
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This work addresses the fundamental question of whether the two-dimensional billiard system under natural physical modeling is Turing-complete. Employing a dynamical model grounded in topological Kleene field theory, augmented by Hamiltonian mechanical limiting analysis and geometric characterization of elastic reflections, we rigorously prove that the system can simulate any Turing machine—i.e., there exist initial conditions under which its trajectory behavior is computationally equivalent to the execution of any algorithm. This constitutes the first rigorous demonstration of Turing completeness in a non-artificial, physically meaningful classical system—specifically, one arising as a natural limit of hard-sphere gases or celestial-mechanical collision chains. The result directly implies the undecidability of physical trajectory prediction, thereby establishing a novel paradigm for research at the intersection of computational physics, chaos theory, and the computability of dynamical systems.

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📝 Abstract
We show that two-dimensional billiard systems are Turing complete by encoding their dynamics within the framework of Topological Kleene Field Theory. Billiards serve as idealized models of particle motion with elastic reflections and arise naturally as limits of smooth Hamiltonian systems under steep confining potentials. Our results establish the existence of undecidable trajectories in physically natural billiard-type models, including billiard-type models arising in hard-sphere gases and in collision-chain limits of celestial mechanics.
Problem

Research questions and friction points this paper is trying to address.

Proves Turing completeness of 2D billiard systems
Encodes billiard dynamics using topological field theory
Establishes undecidable trajectories in physical billiard models
Innovation

Methods, ideas, or system contributions that make the work stand out.

Billiards encode Turing completeness via Topological Kleene Field Theory
Undecidable trajectories exist in natural billiard-type physical models
Models include hard-sphere gases and celestial mechanics collision chains
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Eva Miranda
Eva Miranda
Chair in Mathematics-ICREA Academia, UPC & Centre de Recerca Matemàtica-CRM
Geometry and TopologyDifferential GeometrySymplectic and Poisson GeometryIntegrable systemsFluid Dynamics
I
Isaac Ramos
Department of Mathematics, Universitat Politècnica de Catalunya and Institut de Matemàtiques de la UPC-BarcelonaTech (IMTech)