Laplace Transform Methods for PDEs

How does heat move down a long metal rod when you suddenly heat one end at time zero? This is exactly the kind of question where the Fourier Transform Methods for PDEs toolkit runs into a wall. That toolkit is built for problems on the whole line or with periodic data. Real experiments live on a half-line or finite interval. They start at a definite instant. They have boundary conditions imposed for all future time. The Laplace transform is the natural answer. It is designed precisely for functions defined on t≥0t \ge 0. It converts initial-value problems in time into algebraic or ordinary differential problems in a complex frequency variable ss. The idea generalizes what you already know from ODEs. Transforming ∂t\partial_t into multiplication by ss (minus initial data) turns a linear PDE into an ODE. That ODE is in the spatial variable, parametrized by ss. Solve that ODE, impose the spatial boundary conditions. Then invert the transform to recover u(x,t)u(x,t). This works cleanly for the heat equation, the wave equation on a half-line, and many diffusion-convection-reaction models. It is the standard route to explicit formulas involving the complementary error function and Duhamel-type convolution integrals. The big picture is a trade of one hard problem for two easier ones. First, an algebraic/ODE problem in (x,s)(x,s). Second, a complex contour integral (the Bromwich inversion) to get back to (x,t)(x,t). In practice the inversion step is often bypassed using tables, the convolution theorem, or asymptotic methods. But knowing that the rigorous inversion exists — and under what hypotheses — matters greatly. That is what makes the whole method trustworthy rather than a bag of tricks. This article gives the precise definition of the Laplace transform in time for a PDE. It states and proves the transform rules needed (differentiation, shifting, convolution). It proves the Bromwich inversion theorem under a clean hypothesis set. It carries a full worked solution of the heat equation on a semi-infinite rod. This worked solution proceeds through to the classical error-function answer.

Key takeaways
  • The Laplace transform in tt turns ∂tu\partial_t u into sU−u(x,0)sU - u(x,0), converting an evolution PDE into an ODE (or algebraic equation) in xx, parametrized by s∈Cs\in\mathbb{C}.
  • It is the natural tool when the time domain is t≥0t\ge 0 with prescribed initial data and boundary conditions imposed for all t>0t>0 — unlike Fourier Transform Methods for PDEs, which prefers the whole line or periodicity.
  • Solving the transformed ODE plus boundedness/boundary conditions gives U(x,s)U(x,s) explicitly; recovering u(x,t)u(x,t) is the Bromwich (Mellin) inversion integral, a contour integral in the complex ss-plane.
  • For the heat equation on a half-line with constant boundary temperature, this machinery reproduces the classical error-function solution exactly and rigorously.
  • The method requires functions of at most exponential growth in tt (transform existence) and analytic continuation of U(x,s)U(x,s) to a right half-plane; dropping this breaks invertibility.
  • It sits between d'Alembert's Solution of the Wave Equation (explicit, transform-free) and the general theory of Well-Posedness of PDE Problems, which asks whether such solutions are unique and stable.
  • Key idea: transform time away, solve an ODE in space, then invert a complex contour integral to restore the time dependence.

Where this lives today

Laplace-transform methods for PDEs are the standard classical technique for heat conduction with time-dependent boundary flux or temperature in engineering heat-transfer texts, giving explicit error-function and convolution solutions used in metallurgy and building-thermal design. In electrical engineering and control theory, the same method (there usually applied to the telegrapher's/transmission-line equations, a damped wave equation) computes voltage and current transients on cables and is the origin of the "operational calculus" still taught alongside transfer functions and Laplace-domain circuit analysis. In financial mathematics, Laplace transforms in time solve the Black-Scholes PDE and related barrier-option problems, where the inversion integral becomes a contour integral evaluated by residues or numerical inverse-Laplace algorithms (e.g. the Talbot or Stehfest methods). In numerical analysis, this same viewpoint underlies "Laplace transform methods for evolution equations" used to solve stiff parabolic PDEs by evaluating the resolvent (A−sI)−1(\mathcal A - sI)^{-1} at a handful of contour points rather than time-stepping — a technique tied to semigroup theory and functional-analytic treatments of Well-Posedness of PDE Problems. Finally, the transform's algebraic manipulation of differential operators (turning ∂t\partial_t into ss) is the direct ancestor of the symbolic "operator calculus" used throughout applied mathematics and signal processing, complementing the Fourier Transform Methods for PDEs used for spatial or periodic-in-time problems.

Ask the tutor: How does the choice of branch for s\sqrt{s} in U(x,s)=G(s)e−xs/kU(x,s)=G(s)e^{-x\sqrt{s/k}} affect the validity of the Bromwich inversion contour?

DefinitionLaplace transform of a function of (x,t)(x,t), and its use for evolution PDEs

Let u(x,t)u(x,t) be defined for xx in a spatial domain Ω⊂R\Omega \subset \mathbb{R} and t≥0t \ge 0. Suppose that for each fixed xx, the function t↦u(x,t)t \mapsto u(x,t) is piecewise continuous on [0,∞)[0,\infty) and of exponential order γ\gamma: there exist constants M>0M>0, γ∈R\gamma \in \mathbb{R} such that

∣u(x,t)∣≤Meγtfor all t≥0.|u(x,t)| \le M e^{\gamma t} \qquad \text{for all } t \ge 0.

The Laplace transform of uu in time is the function

U(x,s)  =  L{u}(x,s)  =  ∫0∞e−st u(x,t) dt,U(x,s) \;=\; \mathcal{L}\{u\}(x,s) \;=\; \int_0^\infty e^{-st}\, u(x,t)\, dt,

defined for all complex ss with Re⁡(s)>γ\operatorname{Re}(s) > \gamma, on which the integral converges absolutely. To apply this to a linear evolution PDE

∂tu=Au,u(x,0)=f(x),\partial_t u = \mathcal{A}u, \qquad u(x,0) = f(x),

where A\mathcal{A} is a linear spatial differential operator (e.g. Au=k uxx\mathcal{A}u = k\,u_{xx}), one transforms the equation in tt for each fixed ss with Re⁡(s)>γ\operatorname{Re}(s) > \gamma, obtaining an ordinary differential equation in xx for U(x,s)U(x,s), together with transformed boundary conditions. Solving this subsidiary equation and inverting the transform recovers u(x,t)u(x,t).

Intuition

Think of the Laplace transform as a weighted "totaling up" of a signal's future: multiplying u(x,t)u(x,t) by the decaying exponential e−ste^{-st} and integrating over all t≥0t \ge 0 produces a single number (for each xx and ss) that packages the whole time history. Differentiating in tt becomes, after integration by parts, multiplication by ss — but with a correction term that is exactly the initial data u(x,0)u(x,0). This is the miracle that makes initial-value problems tractable: the transform automatically carries the initial condition into the algebra. Geometrically, picture u(x,t)u(x,t) as a stack of time-signals, one for each xx. The transform flattens each vertical time-slice into a complex number U(x,s)U(x,s), turning a genuinely two-variable PDE into a family of ODEs in xx, one for each value of ss in a right half-plane of the complex plane. Solving that ODE with the spatial boundary data pins down U(x,s)U(x,s) completely as a function of ss (often involving s\sqrt{s} or e−xs/ke^{-x\sqrt{s/k}} for diffusion problems). The final step, recovering u(x,t)u(x,t) from U(x,s)U(x,s), is not a simple algebraic reversal — it requires integrating U(x,s)estU(x,s)e^{st} along a vertical line in the complex plane far enough to the right that UU is analytic, then closing or deforming the contour.

Figure
The Bromwich contour: a vertical line Re⁡(s)=c\operatorname{Re}(s)=c to the right of all singularities of U(x,s)U(x,s)
Re(s) Im(s) c + i∞ c − i∞ Re(s) = c singularities of U(x,s) all singularities lie left of the contour

Setting up the ODE in space

For concreteness, fix the heat equation ut=kuxxu_t = k u_{xx} on x>0x>0, t>0t>0, with u(x,0)=0u(x,0)=0 and u(0,t)=g(t)u(0,t)=g(t). Transforming in tt and writing U(x,s)=L{u}(x,s)U(x,s)=\mathcal L\{u\}(x,s), G(s)=L{g}(s)G(s) = \mathcal L\{g\}(s), the equation becomes the ODE sU=kUxxsU = kU_{xx}, i.e.

Uxx−skU=0,U(0,s)=G(s),U_{xx} - \frac{s}{k}U = 0, \qquad U(0,s) = G(s),

with general solution U(x,s)=A(s)e−xs/k+B(s)exs/kU(x,s) = A(s)e^{-x\sqrt{s/k}} + B(s)e^{x\sqrt{s/k}} (principal branch, Re⁡s/k>0\operatorname{Re}\sqrt{s/k}>0 for Re⁡(s)>0\operatorname{Re}(s)>0). Boundedness as x→∞x\to\infty forces B(s)=0B(s)=0, and the boundary condition gives A(s)=G(s)A(s)=G(s), so

U(x,s)=G(s) e−xs/k.U(x,s) = G(s)\, e^{-x\sqrt{s/k}}.

Inverting this transform is exactly what the theorem below makes rigorous.

TheoremTransform rules and the Bromwich inversion theorem

Part 1 (Transform of the time-derivative). Let u(x,⋅)u(x,\cdot) be continuous on [0,∞)[0,\infty), piecewise C1C^1, of exponential order γ\gamma, with ut(x,⋅)u_t(x,\cdot) also piecewise continuous of exponential order γ\gamma. Then for Re⁡(s)>γ\operatorname{Re}(s)>\gamma,

L{ut}(x,s)=s U(x,s)−u(x,0).\mathcal{L}\{u_t\}(x,s) = s\,U(x,s) - u(x,0).

More generally, if u,ut,…,ut(n−1)u,u_t,\dots,u_t^{(n-1)} are continuous of exponential order γ\gamma and ut(n)u_t^{(n)} is piecewise continuous of exponential order γ\gamma,

L{∂tnu}(x,s)=snU(x,s)−∑j=0n−1sn−1−j ∂tju(x,0).\mathcal{L}\{\partial_t^n u\}(x,s) = s^n U(x,s) - \sum_{j=0}^{n-1} s^{n-1-j}\,\partial_t^j u(x,0).

Part 2 (Uniqueness / injectivity). If u,vu,v are continuous on [0,∞)[0,\infty) of exponential order and L{u}(s)=L{v}(s)\mathcal{L}\{u\}(s)=\mathcal{L}\{v\}(s) for all ss in some right half-plane, then u≡vu\equiv v on [0,∞)[0,\infty).

Part 3 (Bromwich inversion). Suppose U(s)U(s) is analytic in the half-plane Re⁡(s)>γ\operatorname{Re}(s) > \gamma, and suppose there exist constants c>γc>\gamma, M>0M>0, R0>0R_0>0, and p>1p>1 such that

∣U(s)∣≤M∣s∣pwhenever Re⁡(s)≥c, ∣s∣≥R0.|U(s)| \le \frac{M}{|s|^{p}} \quad \text{whenever } \operatorname{Re}(s) \ge c,\ |s|\ge R_0.

Suppose further U=L{u}U = \mathcal L\{u\} for some continuous function uu of exponential order <c<c. Then for every t>0t>0,

u(t)=12πi∫c−i∞c+i∞estU(s) ds,u(t) = \frac{1}{2\pi i} \int_{c-i\infty}^{c+i\infty} e^{st} U(s)\, ds,

where the integral is taken along the vertical line Re⁡(s)=c\operatorname{Re}(s)=c and converges absolutely; the value is independent of the choice of c>γc>\gamma for which the bound holds.

Proof

Part 1, by direct computation (integration by parts — the standard technique for Laplace differentiation rules). Fix xx and suppress it from notation. On any interval [0,T][0,T] where utu_t is continuous,

∫0Te−stut(t) dt=[e−stu(t)]0T+s∫0Te−stu(t) dt,\int_0^T e^{-st}u_t(t)\,dt = \Big[e^{-st}u(t)\Big]_0^T + s\int_0^T e^{-st}u(t)\,dt,

by integration by parts (valid since uu is continuous and piecewise C1C^1, and any finitely many discontinuities of utu_t split [0,T][0,T] into finitely many subintervals on which this identity holds and the boundary terms at internal points cancel by continuity of uu). Since ∣u(t)∣≤Meγt|u(t)|\le Me^{\gamma t}, for Re⁡(s)>γ\operatorname{Re}(s)>\gamma we have e−sTu(T)→0e^{-sT}u(T)\to 0 as T→∞T\to\infty (because ∣e−sTu(T)∣≤Me−(Re⁡(s)−γ)T→0|e^{-sT}u(T)| \le Me^{-(\operatorname{Re}(s)-\gamma)T}\to0). Letting T→∞T\to\infty,

L{ut}(s)=−u(0)+s U(s)=sU(s)−u(0),\mathcal{L}\{u_t\}(s) = -u(0) + s\,U(s) = sU(s)-u(0),

the integral ∫0∞e−stut dt\int_0^\infty e^{-st}u_t\,dt existing because utu_t is piecewise continuous of exponential order γ\gamma, so its Laplace integral converges absolutely for Re⁡(s)>γ\operatorname{Re}(s)>\gamma. The general case follows by induction: apply the n=1n=1 result to ut(n−1)u_t^{(n-1)} in place of uu, whose Laplace transform is sn−1U−∑j=0n−2sn−2−jut(j)(0)s^{n-1}U - \sum_{j=0}^{n-2}s^{n-2-j}u_t^{(j)}(0) by the inductive hypothesis, then combine.

Part 2. This is a consequence of Part 3 applied constructively, but it is cleaner to prove it directly via the Weierstrass approximation route (the standard technique: reduce to moments). Let w=u−vw = u-v; then ww is continuous, of exponential order γ\gamma, and L{w}(s)=0\mathcal L\{w\}(s)=0 for Re⁡(s)>γ\operatorname{Re}(s)>\gamma. Fix c>γc>\gamma and substitute τ=e−t\tau = e^{-t}, ϕ(τ)=eclog⁡(1/τ) w(−log⁡τ)=τ−cw(−log⁡τ)\phi(\tau) = e^{c\log(1/\tau)}\,w(-\log\tau) = \tau^{-c}w(-\log \tau) for τ∈(0,1]\tau\in(0,1], extended by ϕ(0)=0\phi(0)=0; continuity of ww and the exponential-order bound ∣w(t)∣≤Meγt|w(t)|\le Me^{\gamma t} give ∣ϕ(τ)∣≤Mτγ−c→0|\phi(\tau)| \le M\tau^{\gamma - c}\to 0 as τ→0+\tau\to0^+ (since γ<c\gamma<c), so ϕ\phi extends continuously to [0,1][0,1]. For every integer n≥0n\ge0,

∫01τnϕ(τ) dτ=∫0∞e−(c+n+1)tw(t) dt=L{w}(c+n+1)=0,\int_0^1 \tau^n \phi(\tau)\,d\tau = \int_0^\infty e^{-(c+n+1)t} w(t)\,dt = \mathcal L\{w\}(c+n+1) = 0,

using the substitution t=−log⁡τt=-\log\tau, dτ=−τ dtd\tau = -\tau\,dt. Thus ∫01τnϕ(τ) dτ=0\int_0^1 \tau^n\phi(\tau)\,d\tau=0 for every n≥0n\ge0, so ∫01p(τ)ϕ(τ) dτ=0\int_0^1 p(\tau)\phi(\tau)\,d\tau=0 for every polynomial pp. By the Weierstrass approximation theorem, polynomials are dense in C([0,1])C([0,1]) under the sup norm, so there is a sequence of polynomials pk→ϕp_k\to\phi uniformly on [0,1][0,1]; then

∫01ϕ(τ)2 dτ=lim⁡k→∞∫01pk(τ)ϕ(τ) dτ=0,\int_0^1 \phi(\tau)^2\,d\tau = \lim_{k\to\infty}\int_0^1 p_k(\tau)\phi(\tau)\,d\tau = 0,

since ϕ\phi is bounded and pk→ϕp_k\to \phi uniformly. As ϕ2≥0\phi^2\ge0 is continuous with zero integral, ϕ≡0\phi\equiv0 on [0,1][0,1], hence w≡0w\equiv0 on [0,∞)[0,\infty), i.e. u≡vu\equiv v.

Part 3. This is the classical Bromwich contour / Fourier inversion technique. Write s=c+iξs = c+i\xi along the contour, ds=i dξds = i\,d\xi. Formally, and then justified below,

12πi∫c−i∞c+i∞estU(s) ds=12π∫−∞∞e(c+iξ)tU(c+iξ) dξ.\frac{1}{2\pi i}\int_{c-i\infty}^{c+i\infty} e^{st}U(s)\,ds = \frac{1}{2\pi}\int_{-\infty}^{\infty} e^{(c+i\xi)t} U(c+i\xi)\,d\xi.

Define h(t)=e−ctu(t)h(t) = e^{-ct}u(t) for t≥0t\ge0 and h(t)=0h(t)=0 for t<0t<0; since uu has exponential order <c<c, h∈L1(R)h\in L^1(\mathbb{R}) (because ∣h(t)∣≤Me−(c−γ)t|h(t)| \le Me^{-(c-\gamma)t} for t≥0t\ge0, integrable). Its Fourier transform is

h^(ξ)=∫−∞∞e−iξth(t) dt=∫0∞e−(c+iξ)tu(t) dt=U(c+iξ),\hat h(\xi) = \int_{-\infty}^\infty e^{-i\xi t}h(t)\,dt = \int_0^\infty e^{-(c+i\xi)t}u(t)\,dt = U(c+i\xi),

which is exactly the Laplace transform evaluated on the vertical line — this identifies U(c+iξ)U(c+i\xi) as the ordinary Fourier transform of hh, connecting to Fourier Transform Methods for PDEs. The decay hypothesis ∣U(s)∣≤M/∣s∣p|U(s)|\le M/|s|^p for ∣s∣|s| large on Re⁡(s)≥c\operatorname{Re}(s)\ge c with p>1p>1 gives h^(ξ)=U(c+iξ)=O(∣ξ∣−p)\hat h(\xi) = U(c+i\xi) = O(|\xi|^{-p}) as ∣ξ∣→∞|\xi|\to\infty, hence h^∈L1(R)\hat h \in L^1(\mathbb R). By the Fourier inversion theorem (valid since h^∈L1\hat h\in L^1 and hh is continuous on t>0t>0, and hh is the L1L^1 function whose transform is h^\hat h),

h(t)=12π∫−∞∞eiξth^(ξ) dξfor all t where h is continuous, in particular all t>0.h(t) = \frac{1}{2\pi}\int_{-\infty}^\infty e^{i\xi t}\hat h(\xi)\,d\xi \qquad \text{for all } t \text{ where } h \text{ is continuous, in particular all } t>0.

Substituting back h(t)=e−ctu(t)h(t) = e^{-ct}u(t) and h^(ξ)=U(c+iξ)\hat h(\xi)=U(c+i\xi),

u(t)=ect⋅12π∫−∞∞eiξtU(c+iξ) dξ=12π∫−∞∞e(c+iξ)tU(c+iξ) dξ,u(t) = e^{ct}\cdot \frac{1}{2\pi}\int_{-\infty}^{\infty} e^{i\xi t} U(c+i\xi)\,d\xi = \frac{1}{2\pi}\int_{-\infty}^\infty e^{(c+i\xi)t}U(c+i\xi)\,d\xi,

which is precisely 12πi∫c−i∞c+i∞estU(s) ds\frac{1}{2\pi i}\int_{c-i\infty}^{c+i\infty} e^{st}U(s)\,ds after undoing s=c+iξs=c+i\xi, ds=i dξds=i\,d\xi. Absolute convergence of this integral follows from ∣e(c+iξ)tU(c+iξ)∣=ect∣U(c+iξ)∣=O(ect∣ξ∣−p)|e^{(c+i\xi)t}U(c+i\xi)| = e^{ct}|U(c+i\xi)| = O(e^{ct}|\xi|^{-p}), integrable since p>1p>1. Independence of cc: if c1,c2>γc_1,c_2>\gamma both satisfy the decay hypothesis, both formulas compute u(t)u(t) for the same function uu (the one whose Laplace transform is UU, unique by Part 2), so the two contour integrals agree. This completes the proof. ■\blacksquare

∎

Worked examples

Example 1 — Heat equation on a semi-infinite rod with time-varying boundary temperature. Solve ut=kuxxu_t = k u_{xx} for x>0x>0, t>0t>0, with u(x,0)=0u(x,0)=0, u(0,t)=T0 e−αtu(0,t) = T_0\, e^{-\alpha t} for constants T0>0T_0>0, α>0\alpha>0, and u(x,t)→0u(x,t)\to 0 as x→∞x\to\infty. Step 1 — transform. Since u(x,0)=0u(x,0)=0, Part 1 of the theorem gives L{ut}=sU(x,s)\mathcal L\{u_t\} = sU(x,s), and the PDE becomes sU=kUxxsU = kU_{xx}, i.e. Uxx=(s/k)UU_{xx} = (s/k)U. The boundary data transforms (a standard table entry, L{e−αt}(s)=1/(s+α)\mathcal L\{e^{-\alpha t}\}(s) = 1/(s+\alpha) for Re⁡(s)>−α\operatorname{Re}(s)>-\alpha) to

U(0,s)=T0s+α.U(0,s) = \frac{T_0}{s+\alpha}.

Step 2 — solve the ODE. The bounded solution as x→∞x\to\infty (for Re⁡(s)>0\operatorname{Re}(s)>0, so Re⁡s/k>0\operatorname{Re}\sqrt{s/k}>0) is

U(x,s)=T0s+α e−xs/k.U(x,s) = \frac{T_0}{s+\alpha}\,e^{-x\sqrt{s/k}}.

Step 3 — invert using the shift and known pair. Recall the standard Laplace pair (derivable from the Bromwich integral applied to e−ase^{-a\sqrt s}, or from the known solution of ut=kuxxu_t=ku_{xx} with a Heaviside boundary condition):

L−1{1se−xs/k}(t)=erfc⁡ ⁣(x2kt),erfc⁡(z)=2π∫z∞e−η2dη.\mathcal{L}^{-1}\left\{ \frac{1}{s} e^{-x\sqrt{s/k}} \right\}(t) = \operatorname{erfc}\!\left(\frac{x}{2\sqrt{kt}}\right), \qquad \operatorname{erfc}(z) = \frac{2}{\sqrt\pi}\int_z^\infty e^{-\eta^2}d\eta.

We need e−xs/k/(s+α)e^{-x\sqrt{s/k}}/(s+\alpha), not divided by ss; write it via the derivative form using the known pair

L{x2πkt3e−x2/4kt}(s)=e−xs/k\mathcal L\left\{ \frac{x}{2\sqrt{\pi k t^3}} e^{-x^2/4kt}\right\}(s) = e^{-x\sqrt{s/k}}

(the transform of the heat kernel derivative; this is the standard "Laplace transform of the boundary-flux kernel" table entry), and use the shifting rule together with convolution. By the convolution theorem (itself proved by Fubini on the double integral defining L{p∗q}=L{p}L{q}\mathcal L\{p*q\}=\mathcal L\{p\}\mathcal L\{q\}),

u(x,t)=T0∫0te−α(t−τ)  x2πkτ3e−x2/(4kτ) dτ.u(x,t) = T_0\int_0^t e^{-\alpha(t-\tau)}\; \frac{x}{2\sqrt{\pi k \tau^3}} e^{-x^2/(4k\tau)}\, d\tau.

This is the exact solution as a convolution integral. It can be checked at α=0\alpha = 0: then u(x,t)=T0∫0tx2πkτ3e−x2/4kτdτ=T0erfc⁡ ⁣(x2kt)u(x,t) = T_0\int_0^t \frac{x}{2\sqrt{\pi k\tau^3}}e^{-x^2/4k\tau}d\tau = T_0\operatorname{erfc}\!\left(\frac{x}{2\sqrt{kt}}\right), matching the classical constant-boundary-temperature solution and confirming consistency of the table entries used. As t→∞t\to\infty with xx fixed, u(x,t)→0u(x,t)\to0 since the boundary forcing decays like e−αte^{-\alpha t} and the diffused response inherits that decay — consistent with the exponential order hypothesis used throughout.

Example 2 — First-order transport equation with inflow boundary condition (subsidiary equation is only first order). Solve ut+c ux=0u_t + c\,u_x = 0 for x>0,t>0x>0,t>0 (constant c>0c>0), with u(x,0)=0u(x,0) = 0 and u(0,t)=sin⁡(ωt)u(0,t) = \sin(\omega t). Step 1 — transform in tt. Using Part 1 with u(x,0)=0u(x,0)=0: L{ut}=sU(x,s)\mathcal{L}\{u_t\} = sU(x,s). The PDE becomes the first-order linear ODE in xx

sU+cUx=0⟹Ux=−scU.sU + cU_x = 0 \quad\Longrightarrow\quad U_x = -\frac{s}{c}U.

Step 2 — solve. U(x,s)=U(0,s) e−sx/cU(x,s) = U(0,s)\, e^{-sx/c}. The boundary data transforms via the standard pair L{sin⁡ωt}(s)=ω/(s2+ω2)\mathcal L\{\sin\omega t\}(s) = \omega/(s^2+\omega^2), valid for Re⁡(s)>0\operatorname{Re}(s)>0, so

U(x,s)=ωs2+ω2 e−sx/c.U(x,s) = \frac{\omega}{s^2+\omega^2}\, e^{-sx/c}.

Step 3 — invert using the time-shift (second shifting) theorem. The rule L−1{e−asF(s)}(t)=H(t−a)f(t−a)\mathcal L^{-1}\{e^{-as}F(s)\}(t) = H(t-a) f(t-a), where HH is the Heaviside step function and f=L−1{F}f=\mathcal L^{-1}\{F\} (proved directly: ∫0∞e−stH(t−a)f(t−a) dt=∫a∞e−stf(t−a) dt=e−as∫0∞e−sτf(τ) dτ\int_0^\infty e^{-st}H(t-a)f(t-a)\,dt = \int_a^\infty e^{-st}f(t-a)\,dt = e^{-as}\int_0^\infty e^{-s\tau}f(\tau)\,d\tau by the substitution τ=t−a\tau=t-a), gives with a=x/ca = x/c and f(t)=sin⁡(ωt)f(t)=\sin(\omega t):

u(x,t)=H ⁣(t−xc)sin⁡ ⁣(ω(t−xc)).u(x,t) = H\!\left(t - \tfrac{x}{c}\right)\sin\!\left(\omega\left(t - \tfrac{x}{c}\right)\right).

This is exactly the d'Alembert-type traveling-wave answer: the boundary signal propagates undistorted at speed cc, arriving at position xx at time x/cx/c, echoing d'Alembert's Solution of the Wave Equation though here for a first-order (one-directional) transport equation rather than the second-order wave equation. It can be verified directly by substitution: for t>x/ct>x/c, ∂tu=ωcos⁡(ω(t−x/c))\partial_t u = \omega\cos(\omega(t-x/c)) and ∂xu=−ωc⋅(−1)cos⁡(ω(t−x/c))⋅(−1)\partial_x u = -\tfrac{\omega}{c}\cdot(-1)\cos(\omega(t-x/c))\cdot(-1); carefully, ux=−ωcos⁡(ω(t−x/c))⋅(−1/c)⋅(−1)u_x = -\omega\cos(\omega(t-x/c))\cdot(-1/c) \cdot(-1), and combining ut+cux=ωcos⁡(⋅)−ωcos⁡(⋅)=0u_t + cu_x = \omega\cos(\cdot) - \omega\cos(\cdot) = 0, confirming the PDE, and u(0,t)=H(t)sin⁡(ωt)=sin⁡(ωt)u(0,t)=H(t)\sin(\omega t) = \sin(\omega t) for t>0t>0 as required.

Counterexamplewhy the exponential-order hypothesis cannot be dropped

Consider u(t)=et2u(t) = e^{t^2} for t≥0t \ge 0. This function is continuous, but it is not of exponential order: for any γ\gamma, et2/eγt=et2−γt→∞e^{t^2}/e^{\gamma t} = e^{t^2-\gamma t}\to\infty as t→∞t\to\infty, so no bound ∣u(t)∣≤Meγt|u(t)|\le Me^{\gamma t} holds for any M,γM,\gamma. Consequently the defining integral

∫0∞e−stet2 dt\int_0^\infty e^{-st}e^{t^2}\,dt

diverges for every complex ss (the integrand et2−(Re⁡s)t→∞e^{t^2 - (\operatorname{Re} s)t}\to\infty regardless of Re⁡(s)\operatorname{Re}(s)). So L{u}(s)\mathcal L\{u\}(s) does not exist as a function of ss on any half-plane, and the entire machinery collapses at the first step: there is no U(x,s)U(x,s) to solve an ODE for, no Bromwich contour to write down, and no sense in which "Part 1" or "Part 3" of the theorem could apply. This shows concretely why the hypothesis of exponential order is not a technicality: if a candidate solution of an evolution PDE were to grow super-exponentially in time (which can happen, for instance, for certain ill-posed backward-in-time problems, foreshadowing the issues studied under Well-Posedness of PDE Problems), the Laplace-transform method simply does not apply — there is no algebraic subsidiary equation to solve, and no inversion formula to invoke. The method is only as good as the growth control on the solutions it is applied to.

Scope, edge cases & common traps

SituationWhat to checkCommon pitfall
Spatial domain is a half-lineImpose boundedness/decay as x→∞x\to\infty to kill the growing exponential solutionForgetting to discard B(s)exs/kB(s)e^{x\sqrt{s/k}}, giving an unbounded, non-physical U(x,s)U(x,s)
Time-dependent boundary data g(t)g(t)Confirm gg has a Laplace transform (exponential order) before transformingAssuming L{g}\mathcal L\{g\} exists without checking growth (see counterexample)
Branch of s\sqrt{s} or s/k\sqrt{s/k}Fix the principal branch with Re⁡s/k>0\operatorname{Re}\sqrt{s/k} > 0 for Re⁡(s)>0\operatorname{Re}(s)>0, consistent across the whole right half-planeSign errors from an inconsistent branch choice, producing a spurious blow-up
Inverting via tables vs. Bromwich integralTables are shortcuts for exactly the same Bromwich contour computation; use convolution theorem to combine piecesMultiplying two inverse transforms directly instead of convolving them
Finite interval 0<x<L0<x<LSubsidiary ODE has two boundary conditions (at x=0,Lx=0,L); no boundedness condition needed, get A(s),B(s)A(s),B(s) from linear systemTrying to invert an infinite series of poles (many closely spaced ss-singularities) without justifying term-by-term inversion

The mathematician behind it

Origins · 1 minPierre-Simon Laplace and how this was discovered
PL
Pierre-Simon Laplace
1749-1827 · French mathematician and astronomer, developer of the transform methods and celestial mechanics that bear his name

Laplace worked at the intersection of probability theory, mathematical physics, and celestial mechanics in Napoleonic-era France. He introduced the transform that bears his name in the context of probability generating functions and the theory of differential equations, decades before its systematic use for solving PDEs with initial and boundary data became standard engineering practice in the twentieth century, largely through the work of Oliver Heaviside and later rigorous treatments by mathematicians such as Bromwich and Doetsch.

History
- 1749: Pierre-Simon Laplace born in Beaumont-en-Auge, Normandy.
- 1782-1785: Laplace develops transform techniques in his work on probability and celestial mechanics, the origin of the "Laplace transform."
- 1893: Oliver Heaviside popularizes operational calculus methods for solving differential equations in electrical engineering, closely related to Laplace transform techniques.
- 1916-1917: Thomas John I'Anson Bromwich provides a rigorous complex-analytic foundation for the inversion integral, justifying Heaviside's operational methods.
- 1937: Gustav Doetsch's systematic treatise establishes the Laplace transform as a standard rigorous tool for solving partial differential equations with initial-boundary data.
Why use the Laplace transform instead of the Fourier transform for these problems?

The Fourier transform in tt requires the function to be defined (and typically decaying or bounded) on the whole real line −∞<t<∞-\infty<t<\infty, which is unnatural when a physical process genuinely starts at t=0t=0 with a definite initial condition. The Laplace transform is built for functions on t≥0t\ge0 and automatically incorporates initial data through its differentiation rule L{ut}=sU−u(0)\mathcal L\{u_t\}=sU-u(0). It also only requires exponential growth control rather than absolute integrability, so it applies to a much wider class of physically realistic (even growing) time signals. The two transforms coincide in spirit — both diagonalize ∂t\partial_t — but Laplace is the correct tool whenever "time starts now" and initial conditions matter.

Do I always need to compute the Bromwich contour integral by hand?

No. In practice, most problems are solved by recognizing U(x,s)U(x,s) as built from standard transform pairs (exponentials, powers of ss, s\sqrt s, rational functions) combined via shifting, scaling, and the convolution theorem, all of which are shortcuts derived once and for all from the Bromwich integral. The contour integral is mainly invoked directly when no elementary pair matches, often evaluated via residues if UU has only poles, or via a branch-cut integral if UU involves s\sqrt s (as in diffusion problems), producing integrals like the error function.

What if the transformed boundary condition itself does not have a Laplace transform?

Then the method cannot get started, exactly as illustrated in the counterexample with u(t)=et2u(t)=e^{t^2}. Before transforming, you must verify that all data (initial condition, boundary conditions, and forcing terms) are of exponential order. Most physically reasonable signals — bounded, polynomially growing, or exponentially decaying/growing signals — satisfy this, but pathological super-exponential growth (rare in applications, but possible in artificially constructed or blow-up scenarios) rules the method out entirely.

How does this method handle finite spatial intervals, like 0<x<L0<x<L?

The subsidiary ODE in xx is solved exactly as on the half-line, but now both boundary conditions at x=0x=0 and x=Lx=L are used (instead of one boundary condition plus a boundedness condition at infinity), giving a 2×22\times2 linear system for the two constants in the general solution. The resulting U(x,s)U(x,s) typically has infinitely many poles (at values of ss related to the eigenvalues of the associated Sturm-Liouville problem), and inverting via residues at all these poles reproduces the Fourier/eigenfunction series solution — connecting this method directly to separation-of-variables techniques.

Is the Laplace transform method restricted to linear PDEs?

Yes, in its standard form. The core algebraic trick — L{ut}=sU−u(0)\mathcal L\{u_t\}=sU-u(0) — relies on linearity of the transform and of the differential operator; the transform of a nonlinear term like u2u^2 or uuxuu_x does not reduce to a simple algebraic expression in U(x,s)U(x,s), but instead produces a convolution in ss, which usually makes the subsidiary equation as hard as (or harder than) the original PDE. For genuinely nonlinear evolution equations, other methods (energy estimates, fixed-point/semigroup theory, or specific nonlinear transform tricks like Cole-Hopf for Burgers' equation) are used instead.

How does this relate to well-posedness of the PDE?

Constructing an explicit solution via Laplace transform is a strong existence argument, and the injectivity result (Part 2 of the theorem) supplies uniqueness among solutions of the assumed growth class. Continuous dependence on data (the third pillar of well-posedness) is a separate question, usually addressed by direct energy or maximum-principle estimates rather than by transform algebra; the connections between these solvability arguments and the general framework are developed further under Well-Posedness of PDE Problems.

Can this method fail even when a classical solution exists?

Yes — the method can fail to produce the answer even when a perfectly good solution exists, if the growth or analyticity hypotheses of the inversion theorem are not verified, or if U(x,s)U(x,s) cannot be found in closed form. In such cases the subsidiary ODE may still be solved, but the resulting inversion integral must be evaluated numerically (inverse Laplace transform algorithms such as Talbot's method), or asymptotically for large or small tt, rather than in exact closed form.

Before this

Where this leads