For f∈Cc∞(R3)f\in C_c^\infty(\mathbb R^3), its Newtonian potential is

u(x)=(Γ∗f)(x)=∫R3f(y)4π∣x−y∣ dy.u(x)=(\Gamma*f)(x)=\int_{\mathbb R^3}\frac{f(y)}{4\pi|x-y|}\,dy.

The kernel Γ\Gamma is the .

Equation and regularity

The kernel is locally integrable and the source is compactly supported. Distributional differentiation gives −Δu=f-\Delta u=f. Derivatives can be transferred to ff, making uu smooth and the equality classical. At large ∣x∣|x|, u=O(∣x∣−1)u=O(|x|^{-1}). Other sources require their own convergence conditions; the displayed integral is not automatically finite for every distribution or every integrable function at every point.

References