ConceptComplete

Classification and Separation of Variables

Partial differential equations in physics are classified by their type -- elliptic, parabolic, or hyperbolic -- each corresponding to fundamentally different physical phenomena. Separation of variables reduces PDEs to systems of ODEs, leveraging the symmetry of the domain.


Classification of Second-Order PDEs

Definition6.1Elliptic, Parabolic, and Hyperbolic PDEs

A second-order linear PDE Auxx+2Buxy+Cuyy+⋯=0Au_{xx} + 2Bu_{xy} + Cu_{yy} + \cdots = 0 is classified by the discriminant Δ=B2−AC\Delta = B^2 - AC: elliptic if Δ<0\Delta < 0 (e.g., Laplace equation ∇2u=0\nabla^2 u = 0), parabolic if Δ=0\Delta = 0 (e.g., heat equation ut=αuxxu_t = \alpha u_{xx}), hyperbolic if Δ>0\Delta > 0 (e.g., wave equation utt=c2uxxu_{tt} = c^2 u_{xx}). Each type has distinct well-posedness requirements: elliptic needs boundary conditions, parabolic needs initial + boundary, hyperbolic needs initial conditions on a spacelike surface.

ExampleSeparation of Variables for Laplace's Equation

In spherical coordinates, ∇2u=0\nabla^2 u = 0 separates as u(r,θ,ϕ)=R(r)Θ(θ)Φ(ϕ)u(r,\theta,\phi) = R(r)\Theta(\theta)\Phi(\phi). This yields: Φ′′+m2Φ=0\Phi'' + m^2\Phi = 0 (azimuthal), 1sin⁡θddθ(sin⁡θΘ′)+[ℓ(ℓ+1)−m2/sin⁡2θ]Θ=0\frac{1}{\sin\theta}\frac{d}{d\theta}(\sin\theta\Theta') + [\ell(\ell+1) - m^2/\sin^2\theta]\Theta = 0 (associated Legendre), and r2R′′+2rR′−ℓ(ℓ+1)R=0r^2R'' + 2rR' - \ell(\ell+1)R = 0 (Euler-type). Solutions: R=Arℓ+Br−(ℓ+1)R = Ar^\ell + Br^{-(\ell+1)}, ΘΦ=Yℓm(θ,ϕ)\Theta\Phi = Y_\ell^m(\theta,\phi) (spherical harmonics).


Green's Functions for PDEs

Definition6.2Green's Function for the Laplacian

The Green's function G(r,r′)G(\mathbf{r}, \mathbf{r}') for −∇2-\nabla^2 on domain Ω\Omega with Dirichlet boundary conditions satisfies −∇2G=δ(r−r′)-\nabla^2 G = \delta(\mathbf{r} - \mathbf{r}') with G∣∂Ω=0G|_{\partial\Omega} = 0. The solution to −∇2u=f-\nabla^2 u = f with u∣∂Ω=gu|_{\partial\Omega} = g is u(r)=∫ΩG(r,r′)f(r′) d3r′+∮∂Ωg(r′)∂G∂n′ dS′u(\mathbf{r}) = \int_\Omega G(\mathbf{r},\mathbf{r}')f(\mathbf{r}')\,d^3r' + \oint_{\partial\Omega} g(\mathbf{r}')\frac{\partial G}{\partial n'}\,dS'. In free space (R3\mathbb{R}^3): G0=1/(4π∣r−r′∣)G_0 = 1/(4\pi|\mathbf{r}-\mathbf{r}'|).

RemarkMethod of Images

For simple geometries, the Green's function is constructed by the method of images: G=G0+HG = G_0 + H where HH is harmonic and chosen so G∣∂Ω=0G|_{\partial\Omega} = 0. For a half-space z>0z > 0: G(r,r′)=14π∣r−r′∣−14π∣r−r′′∣G(\mathbf{r},\mathbf{r}') = \frac{1}{4\pi|\mathbf{r}-\mathbf{r}'|} - \frac{1}{4\pi|\mathbf{r}-\mathbf{r}''|} where r′′\mathbf{r}'' is the mirror image of r′\mathbf{r}' across z=0z = 0.