Poisson's Equation

Laplace's equation describes a steady state with no sources. Add a source — heat generated inside the plate, electric charge filling a region — and the right-hand side is no longer zero. The result is Poisson's equation:

\nabla^2 u = u_{xx} + u_{yy} = f(x, y),

where f is the source density. It is the inhomogeneous cousin of Laplace's equation, and it is everywhere in physics: in electrostatics \nabla^2 \varphi = -\rho/\varepsilon_0 ties the potential to the charge; in gravity \nabla^2 \Phi = 4\pi G\rho ties the field to the mass.

Particular plus homogeneous

Being linear, Poisson's equation yields to the standard split. Find any particular solution u_p with \nabla^2 u_p = f; then the general solution is

u = u_p + u_h, \qquad \nabla^2 u_h = 0,

where u_h is harmonic and chosen so that the total u meets the boundary conditions — exactly the particular-plus-homogeneous idea used for the heat equation. The source sets the interior bulge; the harmonic part bends the whole solution to fit its frame.

On the whole plane, the solution is built from the fundamental solution (the field of a single point source) by superposing one copy for every bit of the source — a convolution with the Green's function. A single positive point source produces a logarithmic potential \frac{1}{2\pi}\ln r in 2-D, the harmonic-away-from-the-source field that diffusion and gravity both obey.