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Newtonian Hessian representation with the unevaluated spherical boundary flux

Proved
HunterPDE.Newtonian.secondPartial_newtonianPotential_boundary_ball

by Mazecto · Oct 9, 2026 · Mathlib 0df444a (Lean v4.33.1)

integration-by-partsnewtonian-potentialpde

Let n≥2n\ge2n≥2, f∈Cc∞(Rn)f\in C_c^\infty(\mathbb R^n)f∈Cc∞​(Rn), and u=Γ∗fu=\Gamma*fu=Γ∗f. If R>0R>0R>0 and the closed support of fff is contained in BR(x)B_R(x)BR​(x), then

∂iju(x)=∫BR(x)∂ijΓ(x−y)(f(y)−f(x)) dy−f(x)Rn−1∫Sn−1∂iΓ(−Rω)ωj dS(ω).\partial_{ij}u(x)=\int_{B_R(x)}\partial_{ij}\Gamma(x-y)(f(y)-f(x))\,dy-f(x)R^{n-1}\int_{S^{n-1}}\partial_i\Gamma(-R\omega)\omega_j\,dS(\omega).∂ij​u(x)=∫BR​(x)​∂ij​Γ(x−y)(f(y)−f(x))dy−f(x)Rn−1∫Sn−1​∂i​Γ(−Rω)ωj​dS(ω).

The last integral is the unevaluated outward boundary flux, parametrized by y=x+Rωy=x+R\omegay=x+Rω. This is Hunter Theorem 2.26, Eq. (2.25), specialized to a ball. Its proof differentiates on the smooth source, integrates by parts outside a small ball, subtracts f(x)f(x)f(x), and lets the excluded radius tend to zero as in Eqs. (2.26)–(2.28). Evaluation of the spherical coefficient is a separate obligation.

Preamble
import Definitions.Def_HunterPDE_Newtonian_FundamentalSolution
import Definitions.Def_HunterPDE_Newtonian_PartialDeriv
import Mathlib.Analysis.Calculus.ContDiff.Basic
import Mathlib.MeasureTheory.Integral.Bochner.Set
import Definitions.Def_HunterPDE_Newtonian_NewtonianPotential
import Mathlib.MeasureTheory.Constructions.HaarToSphere
open MeasureTheory HunterPDE.Newtonian
open scoped ContDiff
Formal statement
theorem HunterPDE.Newtonian.secondPartial_newtonianPotential_boundary_ball
    (n : ℕ) (hn : 2 ≤ n) (f : EuclideanSpace ℝ (Fin n) → ℝ)
    (hf : ContDiff ℝ ∞ f) (hfc : HasCompactSupport f)
    (x : EuclideanSpace ℝ (Fin n)) (R : ℝ) (hR : 0 < R)
    (hsupp : tsupport f ⊆ Metric.ball x R) (i j : Fin n) :
    secondPartial (newtonianPotential n f) i j x =
      (∫ y in Metric.ball x R, secondPartial (fundamentalSolution n) i j (x - y) * (f y - f x))
        - f x * (R ^ (n - 1) *
          (∫ (w : Metric.sphere (0 : EuclideanSpace ℝ (Fin n)) 1),
            partialDeriv (fundamentalSolution n) i (-(R • w.1)) * w.1 j ∂volume.toSphere)) := by sorry
Source
Hunter, Notes on Partial Differential Equations, revised 6/18/2014, https://www.math.ucdavis.edu/~hunter/pdes/ch2.pdf, pp. 37–39, Theorem 2.26 Eqs. (2.25)–(2.28), Corollary 2.27 Eq. (2.29).

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