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Polytopes and $C^0$-Riemannian metrics with positive $h_{\rm top}$

Marcelo R. R. Alves, Matthias Meiwes

TL;DR

This paper addresses extending topological entropy to non-smooth dynamical objects (polytopes, $C^0$-contact forms, and $C^0$-Riemannian metrics) by introducing entropy notions via star-shaped smoothings. Using the $C^0$-robust positive entropy results from ADMP on $(S^3,\xi_{\rm tight})$, the authors embed smoothed polytopes into a Weinstein neighborhood to transfer lower bounds to the Reeb flows. They prove the main theorem: there exist starshaped polytopes $P\subset \mathbb{R}^4$ such that every star-shaped smoothing of $\partial P$ yields $h_{\rm top} > 0$, and similarly construct non-differentiable $C^0$-forms with arbitrarily large entropy. These results answer Ostrover–Ginzburg and reveal how combinatorial polygonal data relate to chaotic Reeb/geodesic dynamics, while proposing open questions about realization sets and connections to $C^0$-symplectic topology.

Abstract

We study Reeb dynamics on starshaped hypersurfaces in $\mathbb{R}^4$ arising as smoothings of convex polytopes. Using the $C^0$--stability of positive topological entropy for Reeb flows in dimension three from our joint work with Dahinden and Pirnapasov, we show that there exist starshaped polytopes $P$ such that for any starshaped smoothing of $\partial P$ the associated Reeb flows have positive topological entropy. This answers a question of Ostrover and Ginzburg. Similarly, we show that given a closed surface $M$ and a number $C>0$, there exist continuous and non-differentiable Riemannian metrics $g$ on $S$ with $h_{\rm top}>C$ in the sense that for any smoothing of $g$ the associated geodesic flows have $h_{\rm top}>C$.

Polytopes and $C^0$-Riemannian metrics with positive $h_{\rm top}$

TL;DR

This paper addresses extending topological entropy to non-smooth dynamical objects (polytopes, -contact forms, and -Riemannian metrics) by introducing entropy notions via star-shaped smoothings. Using the -robust positive entropy results from ADMP on , the authors embed smoothed polytopes into a Weinstein neighborhood to transfer lower bounds to the Reeb flows. They prove the main theorem: there exist starshaped polytopes such that every star-shaped smoothing of yields , and similarly construct non-differentiable -forms with arbitrarily large entropy. These results answer Ostrover–Ginzburg and reveal how combinatorial polygonal data relate to chaotic Reeb/geodesic dynamics, while proposing open questions about realization sets and connections to -symplectic topology.

Abstract

We study Reeb dynamics on starshaped hypersurfaces in arising as smoothings of convex polytopes. Using the --stability of positive topological entropy for Reeb flows in dimension three from our joint work with Dahinden and Pirnapasov, we show that there exist starshaped polytopes such that for any starshaped smoothing of the associated Reeb flows have positive topological entropy. This answers a question of Ostrover and Ginzburg. Similarly, we show that given a closed surface and a number , there exist continuous and non-differentiable Riemannian metrics on with in the sense that for any smoothing of the associated geodesic flows have .
Paper Structure (5 sections, 3 theorems, 17 equations)

This paper contains 5 sections, 3 theorems, 17 equations.

Key Result

Theorem 1.7

There exist starshaped polytopes $P\subset \mathbbm{R}^4$ such that for any starshaped smoothing $\widetilde{M}$ of $\partial P$, the Reeb flow on $\widetilde{M}$ has positive topological entropy.

Theorems & Definitions (11)

  • Definition 1.1
  • Remark 1.2
  • Definition 1.3
  • Remark 1.4
  • Definition 1.5
  • Remark 1.6
  • Theorem 1.7
  • Theorem 1.8
  • Lemma 1.9
  • proof
  • ...and 1 more