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LeanPool.CaffarelliKohnNirenberg.Foundation.Harmonic.Interior

Interior #

Part of the Caffarelli–Kohn–Nirenberg partial regularity proof.

Harmonic interior estimates from the Newtonian representation #

Kernel and integration-by-parts infrastructure for the representation route.

theorem CKN.Foundation.Heat.spatialDeriv_kernelCutoffDerivative_at_x {x x₀ : Parabolic.Vec3} {ρ : ℝ} (hρ : 0 < ρ) (hx : x ∈ euclideanBall x₀ (13 * ρ / 20)) (i j : Fin 3) :
theorem CKN.Foundation.Heat.spatialDeriv_kernelCutoffDerivative_of_ne {x x₀ y : Parabolic.Vec3} {ρ : ℝ} (hρ : 0 < ρ) (hxy : x - y ≠ 0) (i j : Fin 3) :
spatialDeriv (kernelCutoffDerivative x x₀ hρ i) j y = spatialDeriv (fun (z : Parabolic.Vec3) => newtonianKernel (x - z)) j y * spatialDeriv (eta x₀ hρ) i y + newtonianKernel (x - y) * spatialDeriv (spatialDeriv (eta x₀ hρ) i) j y
theorem CKN.Foundation.Heat.kernelCutoffDerivative_contDiff_one (x x₀ : Parabolic.Vec3) {ρ : ℝ} (hρ : 0 < ρ) (hx : x ∈ euclideanBall x₀ (13 * ρ / 20)) (i : Fin 3) :
ContDiff ℝ (↑1) (kernelCutoffDerivative x x₀ hρ i)
theorem CKN.Foundation.Heat.eta_spatialDeriv_contDiff_two_global (x₀ : Parabolic.Vec3) {ρ : ℝ} (hρ : 0 < ρ) (i : Fin 3) :
ContDiff ℝ (↑2) (spatialDeriv (eta x₀ hρ) i)
theorem CKN.Foundation.Heat.smooth_harmonic_annular_representation_on_outer {H : Parabolic.Vec3 → ℝ} (hH : ContDiff ℝ (↑⊤) H) {x₀ : Parabolic.Vec3} {ρ : ℝ} (hρ : 0 < ρ) (hHarm : ∀ y ∈ euclideanBall x₀ (3 * ρ / 4), spatialLaplacian H y = 0) {x : Parabolic.Vec3} (hx : x ∈ euclideanBall x₀ (13 * ρ / 20)) :
H x = (-∫ (y : Parabolic.Vec3), newtonianKernel (x - y) * (H y * spatialLaplacian (eta x₀ hρ) y)) + 2 * ∑ i : Fin 3, ∫ (y : Parabolic.Vec3), H y * spatialDeriv (kernelCutoffDerivative x x₀ hρ i) i y

A smooth harmonic function is represented in an inner ball by the annular terms obtained from the Newtonian representation and a mollified ball cutoff.

theorem CKN.Foundation.Heat.smooth_harmonic_annular_representation {H : Parabolic.Vec3 → ℝ} (hH : ContDiff ℝ (↑⊤) H) {x₀ : Parabolic.Vec3} {ρ : ℝ} (hρ : 0 < ρ) (hHarm : ∀ y ∈ euclideanBall x₀ ρ, spatialLaplacian H y = 0) {x : Parabolic.Vec3} (hx : x ∈ euclideanBall x₀ (ρ / 4)) :
H x = (-∫ (y : Parabolic.Vec3), newtonianKernel (x - y) * (H y * spatialLaplacian (eta x₀ hρ) y)) + 2 * ∑ i : Fin 3, ∫ (y : Parabolic.Vec3), H y * spatialDeriv (kernelCutoffDerivative x x₀ hρ i) i y