On the algorithmic descriptive complexity of attractors in topological dynamics
Cristobal Rojas, Mathieu Sablik
TL;DR
This work develops a computable-analysis framework to quantify the algorithmic descriptive complexity of attractors in topological dynamics, focusing on the three limiting objects: topological, metric, and statistical attractors. It derives general upper bounds: $\Pi_2$-computability for topological/metric attractors and $\Sigma_2$-computability for statistical attractors, with $\Pi_1$-computability under strong attraction; and shows these bounds are tight through explicit symbolic constructions. The authors build computable symbolic systems realizing $\Pi_1$-, $\Pi_2$-, and $\Sigma_2$-complete attractors, including wild attractors with differing complexities across attractor notions. They further demonstrate how to transfer these dynamics to the unit interval via a computable Cantor-set embedding, producing interval maps with corresponding complex attractors. Overall, the paper clarifies how dynamical constraints shape the computability of asymptotic descriptions and provides concrete, computable examples of highly noncomputable attractors within both symbolic and interval settings.
Abstract
We study the computational problem of rigorously describing the asymptotic behaviour of topological dynamical systems up to a finite but arbitrarily small pre-specified error. More precisely, we consider the limit set of a typical orbit, both as a spatial object (attractor set) and as a statistical distribution (physical measure), and prove upper bounds on the computational resources of computing descriptions of these objects with arbitrary accuracy. We also study how these bounds are affected by different dynamical constrains and provide several examples showing that our bounds are sharp in general. In particular, we exhibit a computable interval map having a unique transitive attractor with Cantor set structure supporting a unique physical measure such that both the attractor and the measure are non computable.
