Metric spaces with small rough angles and the rectifiability of rough self-contracting curves

Abstract

The small rough angle (SRA) condition, introduced by Zolotov in arXiv:1804.00234, captures the idea that all angles formed by triples of points in a metric space are small. In the first part of the paper, we develop the theory of metric spaces (X,d) satisfying the SRA(α) condition for some α<1. Given a metric space (X,d) and 0<α<1, the space (X,dα) satisfies the SRA(2α-1) condition. We prove a quantitative converse up to bi-Lipschitz change of the metric. We also consider metric spaces which are SRA(α) free (there exists a uniform upper bound on the cardinality of any SRA(α) subset) or SRA(α) full (there exists an infinite SRA(α) subset). Examples of SRA free spaces include Euclidean spaces, finite-dimensional Alexandrov spaces of non-negative curvature, and Cayley graphs of virtually abelian groups; examples of SRA full spaces include the sub-Riemannian Heisenberg group, Laakso graphs, and Hilbert space. We study the existence or nonexistence of SRA(ε) subsets for 0<ε<2α-1 in metric spaces (X,dα) for 0<α<1. In the second part of the paper, we apply the theory of metric spaces with small rough angles to study the rectifiability of roughly self-contracting curves. In the Euclidean setting, this question was studied by Daniilidis, Deville, and the first author using direct geometric methods. We show that in any SRA(α) free metric space (X,d), there exists λ0 = λ0(α)>0 so that any bounded roughly λ-self-contracting curve in X, λ λ0, is rectifiable. The proof is a generalization and extension of an argument due to Zolotov, who treated the case λ=0, i.e., the rectifiability of self-contracting curves in SRA free spaces.

0

Turn this paper into a full lesson

ArcXiv compiles a staged curriculum from this paper: 8-12 lessons across beginner → advanced, synthesised section guides, visuals, flashcards, a quiz, exercises, and on-demand deep dives per section. Grounded in the abstract, never invented.

Discussion (0)

Sign in to join the discussion.

Loading comments…