The Newtonian kernel is a fundamental solution of -Δ #
For n ≥ 3, the Newtonian kernel Gₙ(x) = (n (n - 2) ωₙ)⁻¹ ‖x‖²⁻ⁿ on ℝⁿ satisfies the
distributional identity -Δ Gₙ = δ₀: for every C² function f with compact support,
∫ x, Δ f x * Gₙ x = -f 0,
and, with the pole moved to a, ∫ x, Δ f x * Gₙ (x - a) = -f a.
The proof has two steps.
- The weak gradient. Integration by parts against
Gₙholds across the pole: for aC¹functiongwith compact support,∫ Gₙ ∂ᵥg = -∫ (∂ᵥGₙ) g. The kernel is replaced by the smooth regularizationsC (‖x‖² + t) ^ ((2 - n) / 2), for which Mathlib's integration by parts applies, andt → 0⁺by dominated convergence: both the regularized kernels and their derivatives are dominated by the kernel and its derivative. In particularGₙis weakly differentiable on every open set with weak derivative its classical one. - The flux. Summing over an orthonormal basis turns
∫ Δ f Gₙinto-∫ ∇Gₙ · ∇f = (n ωₙ)⁻¹ ∫ ‖x‖⁻ⁿ f' x x, and the radial fundamental theorem of calculusTauCeti.integral_norm_rpow_neg_finrank_mul_fderiv_apply_selfevaluates the latter integral as-(n ωₙ) f 0.
The statement and the normalization follow Evans, Partial Differential Equations, Section 2.2.1, Theorem 1, whose Green's-identity argument on the complement of a small ball is replaced here by the two steps above.
Main declarations #
TauCeti.integral_newtonianKernel_mul_fderiv_eq_neg_fderiv_mul: integration by parts against the Newtonian kernel.TauCeti.hasWeakFDerivOn_newtonianKernel: the classical derivative of the kernel is its weak derivative.TauCeti.integral_laplacian_mul_newtonianKernel:-Δ Gₙ = δ₀.TauCeti.integral_laplacian_mul_newtonianKernel_sub: the same identity with the pole ata.
Integration by parts against the Newtonian kernel. For n ≥ 3 and a C¹ function g
with compact support, ∫ Gₙ ∂ᵥg = -∫ (∂ᵥGₙ) g, although Gₙ is singular at the origin.
The Newtonian kernel is weakly differentiable. For n ≥ 3, on every open set the
classical derivative of Gₙ, which exists away from the origin, is a weak derivative of Gₙ.
The Newtonian kernel is a fundamental solution of -Δ. For n ≥ 3 and every C²
function f with compact support on ℝⁿ, ∫ Δ f · Gₙ = -f 0; that is, -Δ Gₙ = δ₀ in the
sense of distributions.
The Newtonian kernel with pole a is a fundamental solution of -Δ. For n ≥ 3 and
every C² function f with compact support on ℝⁿ, ∫ Δ f · Gₙ(· - a) = -f a.