Inverse Mean Curvature Flow of Rotationally Symmetric Hypersurfaces
Abstract
We prove that the Inverse Mean Curvature Flow of a non-star-shaped, mean-convex embedded sphere in with symmetry about an axis and sufficiently long, thick necks exists for all time and homothetically converges to a round sphere as . Our approach is based on a localized version of the parabolic maximum principle. We also present two applications of this result. The first is an extension of the Minkowski inequality to the corresponding non-star-shaped, mean-convex domains in . The second is a connection between IMCF and minimal surface theory. Based on previous work by Meeks and Yau and using foliations by IMCF, we establish embeddedness of the solution to Plateau's problem and a finiteness property of stable immersed minimal disks for certain Jordan curves in .
Keywords
Cite
@article{arxiv.2008.07490,
title = {Inverse Mean Curvature Flow of Rotationally Symmetric Hypersurfaces},
author = {Brian Harvie},
journal= {arXiv preprint arXiv:2008.07490},
year = {2023}
}
Comments
40 pages, 7 figures. This version includes more exposition on rotationally symmetric immersions, some additional applications, and a simpler example of a non-star-shaped admissible initial surface