Counting geodesics on expander surfaces
Benjamin Dozier, Jenya Sapir
TL;DR
The paper investigates the structure of long closed geodesics on expander hyperbolic surfaces of large genus, proving that almost all geodesics with length above $c\sqrt{g}\log g$ are non-simple and that almost all with length above $c g(\log g)^2$ are filling. By transferring Margulis' counting approach to low length scales via flow boxes and employing a uniform spectral gap to obtain effective mixing and multiple mixing, the authors derive an effective prime geodesic theorem and robust global counts from local box-counts. This framework yields sharp bounds on the prevalence of simple geodesics and establishes filling as the typical behavior for sufficiently long geodesics. The results apply to Weil-Petersson random surfaces, random covers, and Brooks-Makover random surfaces, and the techniques bridge graph-based counting with geometric flow dynamics, providing tools for analyzing random high-genus hyperbolic surfaces with uniform spectral gaps.
Abstract
We study properties of typical closed geodesics on expander surfaces of high genus, i.e. closed hyperbolic surfaces with a uniform spectral gap of the Laplacian. Under an additional systole lower bound assumption, we show almost every geodesic of length much greater than $\sqrt{g}\log g$ is non-simple. And we prove almost every closed geodesic of length much greater than $g (\log g)^2$ is filling, i.e. each component of the complement of the geodesic is a topological disc. Our results apply to Weil-Petersson random surfaces, random covers of a fixed surface, and Brooks-Makover random surfaces, since these models are known to have uniform spectral gap asymptotically almost surely. Our proof technique involves adapting Margulis' counting strategy to work at low length scales.
