Determining a Riemannian Metric from Minimal Areas

Abstract

We prove that if $(M,g)$ is a topological 3-ball with a $C^4$-smooth Riemannian metric $g$, and mean-convex boundary $\partial M$ then knowledge of least areas circumscribed by simple closed curves $\gamma \subset \partial M$ uniquely determines the metric $g$, under some additional geometric assumptions. These are that $g$ is either a) $C^3$-close to Euclidean or b) satisfies much weaker geometric conditions which hold when the manifold is to a sufficient degree either thin, or straight. %sufficiently thin. In fact, the least area data that we require is for a much more restricted class of curves $\gamma \subset \partial M$. We also prove a corresponding local result: assuming only that $(M,g)$ has strictly mean convex boundary at a point $p\in \partial M$, we prove that knowledge of the least areas circumscribed by any simple closed curve $\gamma$ in a neighbourhood $U\subset \partial M$ of $p$ uniquely determines the metric near $p$. Additionally, we sketch the proof of a global result with no thin/straight or curvature condition, but assuming the metric admits minimal foliations "from all directions". The proofs rely on finding the metric along a continuous sweep-out of $M$ by area-minimizing surfaces; they bring together ideas from the 2D-Calderón inverse problem, minimal surface theory, and the careful analysis of a system of pseudo-differential equations.

arXiv commentSecond result optimized to a broader class of thin/straight manifolds. 66 pages, 8 figures

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Cited by in corpus (7)

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• Machine Learning Statistical Gravity from Multi-Region Entanglement Entropy
• Building Bulk Geometry from the Tensor Radon Transform
• More of the Bulk from Extremal Area Variations
• Inverse problem of correlation functions in holography
• The bulk-boundary correspondence for the Einstein equations in asymptotically Anti-de Sitter spacetimes
• Holographic geometry/real-space entanglement correspondence and metric reconstruction