Inverse mean curvature flow in complex hyperbolic space
Giuseppe Pipoli

TL;DR
This paper studies the inverse mean curvature flow of star-shaped hypersurfaces in complex hyperbolic space, showing long-term existence, preservation of shape properties, and convergence to a sub-Riemannian sphere with non-constant Webster curvature in some cases.
Contribution
It establishes the long-term behavior and convergence properties of inverse mean curvature flow in complex hyperbolic space, including examples with non-constant Webster curvature.
Findings
Flow exists for all positive time.
Hypersurfaces remain star-shaped and mean convex.
Convergence to a sub-Riemannian sphere with non-constant Webster curvature.
Abstract
We consider the evolution by inverse mean curvature flow of a closed, mean convex and star-shaped hypersurface in the complex hyperbolic space. We prove that the flow is defined for any positive time, the evolving hypersurface stays star-shaped and mean convex. Moreover the induced metric converges, after rescaling, to a conformal multiple of the standard sub- Riemannian metric on the sphere. Finally we show that there exists a family of examples such that the Webster curvature of this sub-Riemannian limit is not constant.
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsGeometric Analysis and Curvature Flows · Geometry and complex manifolds · Advanced Differential Geometry Research
