Newtonian Hessian representation with the unevaluated spherical boundary flux
ProvedHunterPDE.Newtonian.secondPartial_newtonianPotential_boundary_ballintegration-by-partsnewtonian-potentialpde
Let , , and . If and the closed support of is contained in , then
The last integral is the unevaluated outward boundary flux, parametrized by . 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 , 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 sorrySource
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).