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Application: Differential Equations

Big Idea

A fundamental solution EE of a linear operator LL solves LE=δLE = \delta. Once you have it, convolution u=E∗fu = E * f solves Lu=fLu = f for any source ff. This is the continuous analogue of the superposition principle from ODEs: the integral replaces the sum, and δ\delta replaces the basis vectors.

From ODE Superposition to PDE Convolution

In ODEs, if LL is a linear operator and we can solve Lyi=fiLy_i = f_i for individual sources fif_i, then linearity gives L(∑ciyi)=∑cifiL(\sum c_i y_i) = \sum c_i f_i. This is the superposition principle for finite sums.

For PDEs, we replace the finite sum with an integral. Any source ff can be decomposed as a continuous superposition of point sources:

f(x)=∫Rdf(y) δ(x−y) dy.f(x) = \int_{\mathbb{R}^d} f(y)\, \delta(x - y)\, dy.

This is just the sifting property of the delta, but read physically it says: ff is a superposition of impulses δ(⋅−y)\delta(\cdot - y), each weighted by f(y)f(y). If EE is the response to a single impulse at the origin (i.e. LE=δLE = \delta), then by translation E(⋅−y)E(\cdot - y) is the response to an impulse at yy. Superposing all these responses:

u(x)=∫Rdf(y) E(x−y) dy=(E∗f)(x).u(x) = \int_{\mathbb{R}^d} f(y)\, E(x - y)\, dy = (E * f)(x).

Since LL acts on xx and the integral is over yy, linearity gives

Lu(x)=∫Rdf(y) LE(x−y) dy=∫Rdf(y) δ(x−y) dy=f(x).Lu(x) = \int_{\mathbb{R}^d} f(y)\, LE(x - y)\, dy = \int_{\mathbb{R}^d} f(y)\, \delta(x - y)\, dy = f(x).

So u=E∗fu = E * f solves Lu=fLu = f. Convolution with the fundamental solution is the superposition principle, generalized from sums to integrals.

Fundamental Solutions

Definition 1 (Fundamental solution)

Let L=∑∣α∣≤maαDαL = \sum_{|\alpha| \leq m} a_\alpha D^\alpha be a linear partial differential operator with constant coefficients aα∈Ra_\alpha \in \mathbb{R}. A fundamental solution of LL is a distribution E∈D′(Rd)E \in \mathcal{D}'(\mathbb{R}^d) satisfying

LE=δ.LE = \delta.

The equation LE=δLE = \delta is understood in the distributional sense: ⟨LE,φ⟩=⟨δ,φ⟩=φ(0)\langle LE, \varphi \rangle = \langle \delta, \varphi \rangle = \varphi(0) for all φ∈D(Rd)\varphi \in \mathcal{D}(\mathbb{R}^d). By the definition of distributional differentiation, this becomes ⟨E,L∗φ⟩=φ(0)\langle E, L^*\varphi \rangle = \varphi(0), where L∗L^* is the formal adjoint of LL.

Why distributions are essential here. The equation LE=δLE = \delta has no meaning in classical analysis: the right-hand side is not a function. But even the left-hand side is misleading classically. Consider the Laplacian in R3\mathbb{R}^3: the function E(x)=−1/(4π∣x∣)E(x) = -1/(4\pi|x|) satisfies ΔE(x)=0\Delta E(x) = 0 for every x≠0x \neq 0. Pointwise, the Laplacian cannot “see” the singularity at the origin. But as a distribution, EE acts on test functions via integration, and the singularity contributes. When we compute ⟨ΔE,φ⟩=⟨E,Δφ⟩\langle \Delta E, \varphi \rangle = \langle E, \Delta\varphi \rangle and integrate by parts (excising a ball Bε(0)B_\varepsilon(0), applying Green’s identity, taking ε→0\varepsilon \to 0), the boundary terms on the small sphere do not vanish: they converge to φ(0)\varphi(0). That is where the δ\delta comes from. The distributional derivative detects a contribution at the singularity that pointwise differentiation misses entirely.

Example 1 (Fundamental solution of the Laplacian)

The Laplacian Δ=∑i=1d∂i2\Delta = \sum_{i=1}^d \partial_i^2 in Rd\mathbb{R}^d has fundamental solution

E(x)={12∣x∣d=1,12πlog⁡∣x∣d=2,−1d(d−2)ωd ∣x∣2−dd≥3,E(x) = \begin{cases} \dfrac{1}{2}|x| & d = 1, \\[6pt] \dfrac{1}{2\pi}\log|x| & d = 2, \\[6pt] \dfrac{-1}{d(d-2)\omega_d}\,|x|^{2-d} & d \geq 3, \end{cases}

where ωd\omega_d is the volume of the unit ball in Rd\mathbb{R}^d. In three dimensions this gives the familiar E(x)=−14π∣x∣E(x) = -\frac{1}{4\pi|x|}.

Each of these is locally integrable (the singularity at the origin is integrable), so EE defines a regular distribution. The equation ΔE=δ\Delta E = \delta can be verified by integration by parts: for any φ∈D(Rd)\varphi \in \mathcal{D}(\mathbb{R}^d),

⟨ΔE,φ⟩=⟨E,Δφ⟩=∫RdE(x) Δφ(x) dx=φ(0).\langle \Delta E, \varphi \rangle = \langle E, \Delta \varphi \rangle = \int_{\mathbb{R}^d} E(x)\,\Delta\varphi(x)\, dx = \varphi(0).

The last equality uses Green’s second identity on the domain {∣x∣>ε}\{|x| > \varepsilon\} and a careful limit ε→0\varepsilon \to 0.

Example 2 (Fundamental solution of the heat operator)

The heat operator L=∂t−ΔL = \partial_t - \Delta in Rd×(0,∞)\mathbb{R}^d \times (0, \infty) has fundamental solution

E(x,t)=1(4πt)d/2 e−∣x∣2/4t H(t),E(x, t) = \frac{1}{(4\pi t)^{d/2}}\, e^{-|x|^2/4t}\, H(t),

where H(t)H(t) is the Heaviside function. This is the heat kernel: a Gaussian that spreads over time. For any bounded continuous initial condition ff, the convolution

u(x,t)=(E(⋅,t)∗f)(x)=∫Rd1(4πt)d/2 e−∣x−y∣2/4t f(y) dyu(x,t) = (E(\cdot, t) * f)(x) = \int_{\mathbb{R}^d} \frac{1}{(4\pi t)^{d/2}}\, e^{-|x-y|^2/4t}\, f(y)\, dy

solves the initial value problem ∂tu−Δu=0\partial_t u - \Delta u = 0, u(⋅,0)=fu(\cdot, 0) = f.

The Malgrange-Ehrenpreis Theorem

A natural question: does every linear constant-coefficient operator have a fundamental solution? The answer is yes.

Theorem 1 (Malgrange-Ehrenpreis)

Every non-zero linear partial differential operator with constant coefficients

L=∑∣α∣≤maαDα,aα∈R,L = \sum_{|\alpha| \leq m} a_\alpha D^\alpha, \qquad a_\alpha \in \mathbb{R},

has a fundamental solution E∈D′(Rd)E \in \mathcal{D}'(\mathbb{R}^d).

This is a deep existence result, due independently to Malgrange and Ehrenpreis in the 1950s.

Proof 1

(Sketch via Hahn-Banach.) We need a distribution EE satisfying ⟨E,L∗φ⟩=φ(0)\langle E, L^*\varphi \rangle = \varphi(0) for all φ∈D(Rd)\varphi \in \mathcal{D}(\mathbb{R}^d). Define the linear functional

Φ:L∗(D(Rd))→R,Φ(L∗φ)=φ(0).\Phi : L^*\big(\mathcal{D}(\mathbb{R}^d)\big) \to \mathbb{R}, \qquad \Phi(L^*\varphi) = \varphi(0).

This is well-defined on the image of L∗L^* (one must verify that L∗φ=0L^*\varphi = 0 implies φ(0)=0\varphi(0) = 0, which is the hardest part of the proof and requires estimates on L∗L^*). The key analytic step is showing that Φ\Phi is continuous with respect to the topology inherited from D(Rd)\mathcal{D}(\mathbb{R}^d): there exist a compact set KK and constants C,kC, k such that

∣φ(0)∣≤C∥L∗φ∥Ck(K)for all φ∈D(Rd).|\varphi(0)| \leq C \|L^*\varphi\|_{C^k(K)} \qquad \text{for all } \varphi \in \mathcal{D}(\mathbb{R}^d).

This estimate is the heart of the proof. Once it is established, the Hahn-Banach theorem extends Φ\Phi to a continuous linear functional EE on all of D(Rd)\mathcal{D}(\mathbb{R}^d). This EE is a distribution satisfying LE=δLE = \delta.

Structure of the general solution

The fundamental solution EE is a particular solution of Lu=δLu = \delta, just as in ODE theory. The general solution has the familiar form: general = homogeneous + particular.

Proposition 1 (General solution structure)

Let LL be a constant-coefficient operator.

  1. Non-uniqueness of fundamental solutions. If EE is a fundamental solution of LL and w∈D′(Rd)w \in \mathcal{D}'(\mathbb{R}^d) satisfies Lw=0Lw = 0, then E+wE + w is also a fundamental solution.

  2. All fundamental solutions differ by homogeneous solutions. If E1E_1 and E2E_2 are both fundamental solutions (LE1=LE2=δLE_1 = LE_2 = \delta), then L(E1−E2)=0L(E_1 - E_2) = 0, so E1−E2E_1 - E_2 is a solution of the homogeneous equation.

  3. General solution of Lu=fLu = f. If up=E∗fu_p = E * f is a particular solution of Lu=fLu = f, then every distributional solution of Lu=fLu = f has the form u=up+wu = u_p + w where Lw=0Lw = 0.

Proof 2

Parts 1 and 2 follow from linearity: L(E+w)=LE+Lw=δ+0=δL(E + w) = LE + Lw = \delta + 0 = \delta, and L(E1−E2)=LE1−LE2=δ−δ=0L(E_1 - E_2) = LE_1 - LE_2 = \delta - \delta = 0.

For part 3, if Lu=fLu = f and Lup=fLu_p = f, then L(u−up)=0L(u - u_p) = 0, so w=u−upw = u - u_p solves the homogeneous equation.

This is the exact analogue of the ODE theorem: the general solution of a nonhomogeneous linear equation is a particular solution plus the general solution of the homogeneous equation. Distribution theory provides the particular solution via convolution; the homogeneous solutions depend on the specific operator LL and on boundary or initial conditions.

Solving PDEs via Convolution

With a fundamental solution in hand, the superposition argument from the beginning of this section becomes rigorous.

Theorem 2 (Solution by convolution)

Let LL be a constant-coefficient operator with fundamental solution EE. If f∈D(Rd)f \in \mathcal{D}(\mathbb{R}^d) (or more generally, if ff has compact support and the convolution E∗fE * f is well-defined), then

u=E∗fu = E * f

solves Lu=fLu = f in D′(Rd)\mathcal{D}'(\mathbb{R}^d).

Proof 3

By the properties of convolution and distributional differentiation:

Lu=L(E∗f)=(LE)∗f=δ∗f=f,Lu = L(E * f) = (LE) * f = \delta * f = f,

where we used that LL commutes with convolution (since LL has constant coefficients), LE=δLE = \delta, and δ∗f=f\delta * f = f (the delta is the identity for convolution).

This is the distributional realization of the superposition principle: each point yy contributes an impulse response f(y) E(⋅−y)f(y)\, E(\cdot - y), and the integral over all yy assembles the solution.

Example 3 (Solving Poisson’s equation)

Poisson’s equation −Δu=f-\Delta u = f in R3\mathbb{R}^3 has the solution

u(x)=(E∗f)(x)=14π∫R3f(y)∣x−y∣ dy,u(x) = (E * f)(x) = \frac{1}{4\pi} \int_{\mathbb{R}^3} \frac{f(y)}{|x - y|}\, dy,

which is the Newton potential of ff. This is the gravitational (or electrostatic) potential generated by a mass (or charge) density ff.