A second-order operator for horizontal quasiconvexity in the Heisenberg group and application to convexity preserving for horizontal curvature flow
Antoni Kijowski, Qing Liu, Ye Zhang, Xiaodan Zhou
TL;DR
The paper develops a nonlinear second-order operator $L$ for horizontal quasiconvexity in the Heisenberg group ${\mathbb H}$ and shows that $L[f]\ge 0$ in the viscosity sense is necessary for h-quasiconvexity, while $L[f]>0$ is sufficient. It extends the Euclidean Barron–Goebel–Jensen framework to the sub-Riemannian setting, carefully addressing singularities at characteristic points via envelopes $L^*$ and $\overline{L}$. A uniform notion of $h$-quasiconvexity is introduced and linked to preservation under horizontal curvature flow, with a game-theoretic approximation used to construct and control solutions. The paper also provides practical methods to generate admissible initial data (e.g., star-shaped sets via Minkowski-type functionals) and verifies h-quasiconvexity preservation in star-shaped and rotationally symmetric scenarios, advancing PDE-based convexity theory in sub-Riemannian geometry. The results have potential implications for geometric flows and convexity hull constructions in the Heisenberg group, contributing a PDE-based toolkit for sub-Riemannian convexity analysis.
Abstract
This paper is concerned with a PDE approach to horizontally quasiconvex (h-quasiconvex) functions in the Heisenberg group based on a nonlinear second order elliptic operator. We discuss sufficient conditions and necessary conditions for upper semicontinuous, h-quasiconvex functions in terms of the viscosity subsolution to the associated elliptic equation. Since the notion of h-quasiconvexity is equivalent to the horizontal convexity (h-convexity) of the function's sublevel sets, we further adopt these conditions to study the h-convexity preserving property for horizontal curvature flow in the Heisenberg group. Under the comparison principle, we show that the curvature flow starting from a star-shaped h-convex set preserves the h-convexity during the evolution.
