Evolving to Non-round Weingarten Spheres: Integer Linear Hopf Flows
Brendan Guilfoyle, Wilhelm Klingenberg

TL;DR
This paper studies the evolution of rotationally symmetric spheres under specific linear curvature flows, revealing diverse behaviors including convergence to round or non-round Hopf spheres, divergence, and the role of umbilic points.
Contribution
It introduces conditions for evolving spheres via integer coefficient linear flows, linking the fate of the evolution to local umbilic geometry and astigmatism vanishing rates.
Findings
Diverse evolution outcomes depending on flow coefficients.
The size of astigmatism at umbilic points determines sphere fate.
Existence of soliton-like solutions in the curvature flow.
Abstract
In the 1950's Hopf gave examples of non-round convex 2-spheres in Euclidean 3-space with rotational symmetry that satisfy a linear relationship between their principal curvatures. In this paper we investigate conditions under which evolving a smooth rotationally symmetric sphere by a linear combination of its radii of curvature yields a Hopf sphere. When the coefficients of the flow have certain integer values, the fate of an initial sphere is entirely determined by the local geometry of its isolated umbilic points. A surprising variety of behaviours is uncovered: convergence to round spheres and non-round Hopf spheres, as well as divergence to infinity. The critical quantity is the rate of vanishing of the astigmatism - the difference of the radii of curvature - at the isolated umbilic points. It is proven that the size of this quantity versus the coefficient in the flow function…
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