English

Inverse Mean Curvature Flow of Rotationally Symmetric Hypersurfaces

Differential Geometry 2023-03-30 v4 Analysis of PDEs

Abstract

We prove that the Inverse Mean Curvature Flow of a non-star-shaped, mean-convex embedded sphere in Rn+1\mathbb{R}^{n+1} with symmetry about an axis and sufficiently long, thick necks exists for all time and homothetically converges to a round sphere as tt \rightarrow \infty. 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 Rn+1\mathbb{R}^{n+1}. 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 R3\mathbb{R}^{3}.

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