Quasi-spherical metrics and the static Minkowski inequality
Brian Harvie, Ye-Kai Wang
TL;DR
The paper proves a sharp rigidity result for equality in a static Minkowski-type inequality on asymptotically flat manifolds: equality occurs only for slices of Schwarzschild space. It develops a robust framework combining inverse mean curvature flow (IMCF) and quasi-spherical metrics, establishing smoothness of the weak IMCF after a finite time and deriving rotational symmetry of the metric and potential at infinity. Through detailed analysis of the static equations in polar coordinates and careful harmonic-mode expansions, it shows that equality enforces full rotational symmetry and canonical Schwarzschild geometry outside a compact set, with a precise metric form $g= u^{2} dr^{2} + r^{2} g_{S^{n-1}}$ and $V$ solving the static system. The results yield broad applications, including photon-surface uniqueness, static metric extension uniqueness, and higher-dimensional black hole uniqueness, all grounded in a boundary-energy framework and monotonicity of a static Minkowski functional. Overall, the work provides a dimension-agnostic rigidity criterion for Schwarzschild space in the static vacuum setting and advances understanding of quasi-local mass and boundary geometry in general relativity.
Abstract
We prove that equality within the Minkowski inequality for asymptotically flat static manifolds is achieved only by slices of Schwarzschild space.
