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Laplace's equation and harmonic functions

Harmonic functions, radial solutions, the mean value property and its consequences.

A function with \( \Delta u = 0 \) is harmonic. Harmonic functions describe equilibria: the steady temperature in a body, the electrostatic potential in empty space, the velocity potential of an ideal flow. In the plane the real and imaginary parts of every holomorphic function are harmonic, which supplies examples: \( x^2 - y^2 = \operatorname{Re} z^2 \), \( x^3 - 3xy^2 = \operatorname{Re} z^3 \) (the example), \( e^x\cos y = \operatorname{Re} e^z \).

Radial solutions come from \( \Delta u = u_{rr} + \frac{n-1}{r}u_r \) in \( \mathbb R^n \). Setting this to zero gives \( u = a + b\ln r \) in the plane and \( u = a + b\,r^{2-n} \) for \( n \ge 3 \), so \( 1/r \) in space. They are harmonic everywhere except the origin, and that singularity is the seed of the fundamental solution two lessons on.

The central fact is the mean value property: if \( u \) is harmonic on a ball, its value at the centre equals its average over every sphere (and every ball) around that centre. Proof: let \( \phi(r) \) be the average of \( u \) over the sphere of radius \( r \). Differentiating under the integral, \( \phi'(r) \) is the average of the outward normal derivative \( \partial_\nu u \) over that sphere, which by the divergence theorem is a multiple of \( \int_{B_r}\Delta u = 0 \). So \( \phi \) is constant, and as \( r \to 0 \) it tends to \( u \) at the centre.

Picture it: a soap film stretched over a bent wire frame. Each point of the film sits at the average height of any small circle around it; the film has no bumps or dips of its own, only the ones the frame forces on it.

Think it: almost everything about harmonic functions follows from averaging. A harmonic function cannot have an interior maximum unless it is constant (the next lesson). It is infinitely differentiable, because averaging against a smooth bump reproduces it. A harmonic function on all of \( \mathbb R^n \) that is bounded is constant (Liouville), because averages over enormous balls centred at two nearby points almost coincide. In fluid mechanics the pressure solves a Poisson equation \( -\Delta p = \partial_i\partial_j(u_iu_j) \), so these facts are where pressure estimates start.

Ejemplo resuelto · laplacian of x^3 - 3*x*y^2

Laplacian of x^3 - 3*x*y^2

\nabla^2\left(x^{3} - 3 x y^{2}\right)

Paso a paso

  1. f(x, y) = x^{3} - 3 x y^{2},\quad \nabla^2 f = \frac{\partial^2 f}{\partial x^2} + \frac{\partial^2 f}{\partial y^2}

    The Laplacian adds the second partial derivative in each direction.

  2. \frac{\partial f}{\partial x} = 3 x^{2} - 3 y^{2},\quad \frac{\partial^2 f}{\partial x^2} = 6 x

    Differentiate twice with respect to x, holding the other variables constant.

  3. \frac{\partial f}{\partial y} = - 6 x y,\quad \frac{\partial^2 f}{\partial y^2} = - 6 x

    Differentiate twice with respect to y, holding the other variables constant.

  4. \nabla^2 f = \left(6 x\right) + \left(- 6 x\right) = 0

    Add the second partials.

  5. \nabla^2 f = 0

    The Laplacian is zero, so f is harmonic: it solves Laplace's equation.

Revelar la respuesta
\nabla^2 f = 0

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Cómo: Laplace's equation and harmonic functions

  1. Compute each pure second partial derivative and add them.
  2. In the plane, test whether the function is the real or imaginary part of a holomorphic function.
  3. For radial functions use u_rr + (n-1)u_r / r instead of Cartesian derivatives.
  4. Use the mean value property to read off the value at a centre from boundary averages.

Preguntas que la gente hace

Is the product of two harmonic functions harmonic?

Not in general: Δ(uv) = uΔv + vΔu + 2∇u·∇v, and the cross term survives. x and y are harmonic, xy is harmonic, but x times x is not.

What is the difference between Laplace's and Poisson's equation?

Laplace's is Δu = 0; Poisson's is Δu = f with a given source. Their difference is the difference between empty space and space containing charge or mass.

What should I know before starting?

Partial derivatives, the divergence theorem and multiple integrals from multivariable calculus; linear second-order ODEs; eigenvalues from linear algebra; and enough analysis to be comfortable with uniform convergence and integrals over infinite intervals.

Why are there so few formulas for solutions?

Explicit solutions exist for linear equations with constant coefficients on simple domains. Almost everything else (curved domains, variable coefficients, nonlinear terms) has none, so the modern subject proves that a solution exists and estimates its size and smoothness without ever writing it down.

How does this course lead to the Navier-Stokes problem?

The Navier-Stokes equations are a heat equation for the velocity with a transport term and a pressure that is found from a Poisson equation. Reading the Millennium problem needs energy estimates, weak solutions, Sobolev spaces, local existence with a blow-up criterion, and the scaling argument that explains why three dimensions is hard. The last six lessons build those.

What do elliptic, parabolic and hyperbolic mean?

Elliptic equations (Laplace) describe equilibrium and smooth everything; parabolic equations (heat) describe diffusion forward in time; hyperbolic equations (waves) carry signals at finite speed and keep their sharp edges. The type decides which data make a sensible problem.

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