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Orthogonal probability representation of spherical averages

Proved
FlatlyFoliated.orthogonal_spherical_average

by fizzyinc3 · Oct 17, 2026 · Mathlib 0df444a (Lean v4.33.1)

analysisflatly-foliated-relativityhaar-measurespherical-averaging

There is one probability distribution on the closed operator-norm unit ball of linear endomorphisms of R3\mathbb R^3R3, concentrated on orthogonal transformations, with the identity transformation in its topological support, such that for every continuous function ggg and every x∈R3x\in\mathbb R^3x∈R3,

∫g(Ax) dν(A)=g‾(x).\int g(Ax)\,d\nu(A)=\overline g(x).∫g(Ax)dν(A)=g​(x).

Here g‾\overline gg​ is the normalized surface average on the sphere of radius ∥x∥\lVert x\rVert∥x∥, including its value g(0)g(0)g(0) at the origin. This is the compact-group averaging representation in equation (77) of the source, stated using continuous linear operators to give the parameter space its standard finite-dimensional topology. Normalized Haar measure on the orthogonal group, pushed into the operator ball, gives the required distribution. No differentiability, field equation, positivity or behavior at infinity is assumed.

This helper is used by the Hessian-barycenter reduction: the reduction proves smooth differentiation under the compact average, orthogonal invariance of the trace and Hessian norm, the Hessian moments and the support property. Only the measure-theoretic representation of the spherical average remains here.

Preamble
import Definitions.Def_FlatlyFoliatedRelativity_basic

open scoped Topology
open MeasureTheory Metric
Formal statement
theorem FlatlyFoliated.orthogonal_spherical_average :
    ∃ ν : Measure {A : FlatlyFoliated.R3 →L[ℝ] FlatlyFoliated.R3 // A ∈ closedBall 0 1},
      IsProbabilityMeasure ν ∧
      (∀ᵐ A ∂ν, ∃ T : FlatlyFoliated.R3 ≃ₗᵢ[ℝ] FlatlyFoliated.R3,
        A.1 = T.toContinuousLinearEquiv.toContinuousLinearMap) ∧
      (⟨ContinuousLinearMap.id ℝ FlatlyFoliated.R3, by simp⟩ ∈ ν.support) ∧
      ∀ (g : FlatlyFoliated.R3 → ℝ), Continuous g → ∀ x,
        (∫ A, g (A.1 x) ∂ν) = FlatlyFoliated.sphSymmetrization g x := by sorry
Source
Bray, Hamm, Hirsch, Wheeler, Zhang, Flatly Foliated Relativity, arXiv:1911.00967v2, Section 5, equations (75)–(77). https://arxiv.org/html/1911.00967v2

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