Laplacian

Laplacian operator in physical field equations, harmonic potentials, and diffusion processes.

What it is

The Laplacian is a second-order differential operator, denoted by ∇2\nabla^2 or Δ\Delta, defined as the divergence of the gradient:

∇2ϕ=∇⃗⋅(∇⃗ϕ)\nabla^2 \phi = \vec{\nabla} \cdot (\vec{\nabla} \phi)

In Cartesian coordinates it is the sum of pure unmixed second partial derivatives:

∇2ϕ=∂2ϕ∂x2+∂2ϕ∂y2+∂2ϕ∂z2\nabla^2 \phi = \frac{\partial^2 \phi}{\partial x^2} + \frac{\partial^2 \phi}{\partial y^2} + \frac{\partial^2 \phi}{\partial z^2}

Physically, the Laplacian measures the local mean curvature or the difference between the central value of a function and its spherical average in an infinitesimal surrounding neighborhood:

∇2ϕ(P)=lim⁡R→06R2(⟨ϕ⟩SR−ϕ(P))\nabla^2 \phi(P) = \lim_{R \to 0} \frac{6}{R^2} \left( \langle \phi \rangle_{S_R} - \phi(P) \right)

  • If ∇2ϕ(P)>0\nabla^2 \phi(P) > 0: ϕ(P)\phi(P) is smaller than the average of its neighbors (local valley / concave upward).
  • If ∇2ϕ(P)<0\nabla^2 \phi(P) < 0: ϕ(P)\phi(P) is greater than the average of its neighbors (local peak / concave downward).
  • If ∇2ϕ(P)=0\nabla^2 \phi(P) = 0: ϕ(P)\phi(P) matches its neighborhood average identically. Solutions are called harmonic functions.

Why it appears in physics

The Laplacian is the mathematical engine of field equations:

  • Poisson's equation: ∇2V=−ρε0\nabla^2 V = -\frac{\rho}{\varepsilon_0} (electrostatics) and ∇2Φ=4πGρ\nabla^2 \Phi = 4\pi G \rho (gravitation).
  • Laplace's equation: ∇2ϕ=0\nabla^2 \phi = 0. Governs steady-state diffusion, vacuum potentials, and irrotational potential flows.
  • Heat / diffusion equation: ∂T∂t=α∇2T\frac{\partial T}{\partial t} = \alpha \nabla^2 T. Heat flows to eliminate local discrepancies from the mean.
  • Wave equation: ∇2u=1c2∂2u∂t2\nabla^2 u = \frac{1}{c^2} \frac{\partial^2 u}{\partial t^2}. Governs acoustics, light, and seismic waves.
  • Schrödinger equation: −ℏ22m∇2ψ+Vψ=Eψ-\frac{\hbar^2}{2m} \nabla^2 \psi + V \psi = E \psi. Quantum kinetic energy is proportional to the Laplacian of the wavefunction.

Visual or geometric intuition

Picture an elastic drum membrane:

  • When undisturbed, its height profile satisfies Laplace's equation ∇2z=0\nabla^2 z = 0: every point sits at the exact average of its surrounding ring.
  • Under a transverse localized weight, curvature changes non-trivially (∇2z≠0\nabla^2 z \neq 0), modeling Poisson's equation with a point load.

Minimal symbolic language

  • Cartesian coordinates: ∇2=∂xx+∂yy+∂zz\nabla^2 = \partial_{xx} + \partial_{yy} + \partial_{zz}.
  • Cylindrical coordinates: ∇2ϕ=1r∂∂r(r∂ϕ∂r)+1r2∂2ϕ∂θ2+∂2ϕ∂z2\nabla^2 \phi = \frac{1}{r} \frac{\partial}{\partial r}\left(r \frac{\partial \phi}{\partial r}\right) + \frac{1}{r^2} \frac{\partial^2 \phi}{\partial \theta^2} + \frac{\partial^2 \phi}{\partial z^2}.
  • Spherical coordinates: ∇2ϕ=1r2∂∂r(r2∂ϕ∂r)+1r2sin⁡θ∂∂θ(sin⁡θ∂ϕ∂θ)+1r2sin⁡2θ∂2ϕ∂φ2\nabla^2 \phi = \frac{1}{r^2} \frac{\partial}{\partial r}\left(r^2 \frac{\partial \phi}{\partial r}\right) + \frac{1}{r^2 \sin\theta} \frac{\partial}{\partial \theta}\left(\sin\theta \frac{\partial \phi}{\partial \theta}\right) + \frac{1}{r^2 \sin^2\theta} \frac{\partial^2 \phi}{\partial \varphi^2}.
  • Vector Laplacian: ∇2A⃗=∇⃗(∇⃗⋅A⃗)−∇⃗×(∇⃗×A⃗)\nabla^2 \vec{A} = \vec{\nabla}(\vec{\nabla}\cdot\vec{A}) - \vec{\nabla}\times(\vec{\nabla}\times\vec{A}).

What the result means

Non-zero ∇2ϕ\nabla^2 \phi signals that ϕ\phi deviates from local equilibrium. In diffusion, ∇2T>0\nabla^2 T > 0 means the point will warm up; ∇2T<0\nabla^2 T < 0 means it will cool down.

When not to use it

  • Do not use Cartesian second derivatives in polar or spherical systems without metric scale factors.
  • For vector fields in curvilinear coordinates, do not take the Laplacian component-by-component because unit vectors rotate with position. Use ∇2A⃗=∇⃗(∇⃗⋅A⃗)−∇⃗×(∇⃗×A⃗)\nabla^2 \vec{A} = \vec{\nabla}(\vec{\nabla}\cdot\vec{A}) - \vec{\nabla}\times(\vec{\nabla}\times\vec{A}).

Operational summary

To compute ∇2ϕ\nabla^2 \phi: evaluate second partial derivatives and sum them. If ∇2ϕ=0\nabla^2 \phi = 0, the function obeys the mean-value property and has no local extrema in the interior (Earnshaw's theorem).

Procedure

Before calculating

Confirm whether the input is a scalar field ϕ\phi or a vector field A⃗\vec{A} and select the optimal coordinate system.

Step 1: Identify the mathematical object

Formulate the target equation: Laplace (∇2ϕ=0\nabla^2 \phi = 0), Poisson, diffusion, or Helmholtz.

Step 2: Choose the operation

Select the appropriate Laplacian formula:

  • Cartesian: ∂xxϕ+∂yyϕ+∂zzϕ\partial_{xx} \phi + \partial_{yy} \phi + \partial_{zz} \phi.
  • Cylindrical: 1r∂r(r∂rϕ)+1r2∂θ2ϕ+∂z2ϕ\frac{1}{r}\partial_r(r\partial_r \phi) + \frac{1}{r^2}\partial_\theta^2 \phi + \partial_z^2 \phi.
  • Spherical: 1r2∂r(r2∂rϕ)+1r2sin⁡θ∂θ(sin⁡θ∂θϕ)+1r2sin⁡2θ∂φ2ϕ\frac{1}{r^2}\partial_r(r^2\partial_r \phi) + \frac{1}{r^2\sin\theta}\partial_\theta(\sin\theta\partial_\theta \phi) + \frac{1}{r^2\sin^2\theta}\partial_\varphi^2 \phi.

Step 3: Conserve units and signs

Perform inner first derivatives, multiply by coordinate scale weights, then evaluate outer derivatives.

Step 4: Calculate

Combine all terms and simplify. Substitute spatial coordinates for numerical evaluations.

Step 5: Interpret the result

Interpret physical significance: ∇2ϕ=0\nabla^2 \phi = 0 indicates harmonic equilibrium; non-zero values reveal local source density or diffusion rates.

Self-check checklist

  • Is the output for a scalar field a scalar?
  • Were curvilinear scale weights differentiated correctly?
  • Are dimensions [ϕ]/[m2][\phi]/[\text{m}^2]?

Guided example

Physical situation

An infinitely long coaxial cable consists of an inner core of radius a=1.0 mma = 1.0 \text{ mm} held at voltage Va=100 VV_a = 100 \text{ V} and an outer shield of radius b=5.0 mmb = 5.0 \text{ mm} grounded at Vb=0 VV_b = 0 \text{ V}. Space between (a<r<ba < r < b) is vacuum.

  1. Solve Laplace's equation ∇2V=0\nabla^2 V = 0 for V(r)V(r).
  2. Calculate electric field E⃗(r)=−∇⃗V\vec{E}(r) = -\vec{\nabla} V.

Mathematical translation

By cylindrical symmetry: V=V(r)V = V(r). ∇2V=1rddr(rdVdr)=0\nabla^2 V = \frac{1}{r} \frac{d}{dr}\left( r \frac{dV}{dr} \right) = 0

Step-by-step calculation

  1. Integrate ODE: rdVdr=C1  ⟹  dVdr=C1r  ⟹  V(r)=C1ln⁡(r)+C2r \frac{dV}{dr} = C_1 \implies \frac{dV}{dr} = \frac{C_1}{r} \implies V(r) = C_1 \ln(r) + C_2

  2. Impose boundary conditions: V(a)=VaV(a) = V_a and V(b)=0V(b) = 0: C1=−Valn⁡(b/a),C2=Valn⁡(b)ln⁡(b/a)C_1 = -\frac{V_a}{\ln(b/a)}, \quad C_2 = \frac{V_a \ln(b)}{\ln(b/a)} V(r)=Valn⁡(b/r)ln⁡(b/a)V(r) = V_a \frac{\ln(b/r)}{\ln(b/a)}

  3. Numerical evaluation (Va=100 V,b/a=5V_a = 100\text{ V}, b/a = 5): V(r)=100ln⁡(0.005/r)ln⁡(5)≈62.133ln⁡(0.005/r)[V]V(r) = 100 \frac{\ln(0.005/r)}{\ln(5)} \approx 62.133 \ln(0.005/r) \quad [\text{V}]

  4. Electric field: E⃗(r)=−dVdre^r=Varln⁡(b/a)e^r=62.133re^r[V/m]\vec{E}(r) = -\frac{dV}{dr} \hat{e}_r = \frac{V_a}{r \ln(b/a)} \hat{e}_r = \frac{62.133}{r} \hat{e}_r \quad [\text{V/m}] At r=a=10−3 mr = a = 10^{-3}\text{ m}: E(a)≈62.13 kV/mE(a) \approx 62.13 \text{ kV/m}.

Reading the result

Potential falls off logarithmically and field scales as 1/r1/r. Zero Laplacian confirms charge-free dielectric space.

Common error avoided

Using Cartesian d2Vdr2=0\frac{d^2 V}{dr^2} = 0, which yields an invalid linear profile.


Inverse example

Given result

A spherical cloud yields a constant Laplacian ∇2V=−K\nabla^2 V = -K inside r<Rr < R.

What physical question it can answer

What is the internal charge density? By Poisson's equation ∇2V=−ρ/ε0  ⟹  ρ=Kε0\nabla^2 V = -\rho / \varepsilon_0 \implies \rho = K \varepsilon_0. The constant Laplacian proves the sphere contains a perfectly uniform charge distribution.

Common errors

Error 1: Conflating the Laplacian with squared gradient magnitude

Confusing ∇2ϕ\nabla^2 \phi with ∥∇⃗ϕ∥2\|\vec{\nabla}\phi\|^2. The Laplacian is a linear sum of second derivatives, whereas the squared gradient norm is a nonlinear product of squared first derivatives.

Error 2: Omitting curvilinear metric curvature terms

Evaluating the spherical radial Laplacian as merely ∂rrϕ\partial_{rr} \phi. The correct radial term is ∂rrϕ+2r∂rϕ\partial_{rr}\phi + \frac{2}{r}\partial_r\phi. Neglecting 2r∂r\frac{2}{r}\partial_r invalidates the physical solution.

Error 3: Taking component-wise Laplacians in curvilinear vector fields

Writing ∇2A⃗=∑i(∇2Ai)e^i\nabla^2 \vec{A} = \sum_i (\nabla^2 A_i) \hat{e}_i in spherical or cylindrical frames. Curvilinear unit vectors rotate with coordinates; one must use ∇2A⃗=∇⃗(∇⃗⋅A⃗)−∇⃗×(∇⃗×A⃗)\nabla^2 \vec{A} = \vec{\nabla}(\vec{\nabla}\cdot\vec{A}) - \vec{\nabla}\times(\vec{\nabla}\times\vec{A}).

Error 4: Expecting local extrema inside harmonic domains

Searching for electrostatic traps for free charged particles in vacuum. Earnshaw's theorem states that because ∇2V=0\nabla^2 V = 0, stable isolated potential minima cannot exist in source-free space.

Error 5: Surprised that linear functions have zero Laplacian

Overlooking that any linear function ax+by+cz+da x + b y + c z + d trivially satisfies Laplace's equation.

Quick detection rule

If a Laplacian formula contains cross derivatives ∂xy\partial_{xy} in Cartesian frames, or fails to carry physical units of [ϕ]/[m2][\phi]/[\text{m}^2], it is mathematically incorrect.

Physical applications

1. Electrostatics and gravity: Poisson and Laplace formulations

  • ∇2V=−ρ/ε0\nabla^2 V = -\rho/\varepsilon_0 (Coulomb potential).
  • ∇2Φ=4πGρ\nabla^2 \Phi = 4\pi G \rho (Newtonian gravity).
  • ∇2V=0\nabla^2 V = 0 in vacuum (Earnshaw's theorem forbidding static charge traps).

2. Quantum mechanics: Schrödinger wave mechanics

The kinetic energy operator is T^=−ℏ22m∇2\hat{T} = -\frac{\hbar^2}{2m} \nabla^2. The Laplacian dictates hydrogen atomic orbitals, solid-state electronic band structures, and tunneling.

3. Heat conduction and molecular diffusion

Fourier's heat equation ∂tT=α∇2T\partial_t T = \alpha \nabla^2 T and Fick's second law ∂tc=D∇2c\partial_t c = D \nabla^2 c describe relaxation toward maximum entropy.

4. Acoustics, optics, and electrodynamic waves

The d'Alembert wave equation ∇2u−1c2∂ttu=0\nabla^2 u - \frac{1}{c^2} \partial_{tt} u = 0 governs sound propagation, seismic waves, and electromagnetic light waves.

5. Elasticity and plate mechanics

Transverse deflections of elastic thin plates under load satisfy the biharmonic equation ∇4w=∇2(∇2w)=q/D\nabla^4 w = \nabla^2(\nabla^2 w) = q/D.

Practice

Problem 1: Mean value theorem and harmonic functions

Test if V(x,y)=excos⁡(y)+3xyV(x,y) = e^x \cos(y) + 3xy is harmonic by evaluating ∇2V\nabla^2 V.

Solution:

∂xxV=excos⁡y,∂yyV=−excos⁡y\partial_{xx} V = e^x \cos y, \quad \partial_{yy} V = -e^x \cos y ∇2V=excos⁡y−excos⁡y=0\nabla^2 V = e^x \cos y - e^x \cos y = 0 The function is harmonic on R2\mathbb{R}^2. By Earnshaw's theorem, it admits no isolated local maxima or minima.


Problem 2: Poisson's equation and electron cloud density

Electrostatic potential is V(r)=e4πε0e−2r/a0rV(r) = \frac{e}{4\pi\varepsilon_0} \frac{e^{-2r/a_0}}{r}. Compute ∇2V\nabla^2 V for r>0r > 0 and find ρ(r)\rho(r).

Solution:

Using ∇2V=1rd2dr2(rV)\nabla^2 V = \frac{1}{r}\frac{d^2}{dr^2}(rV): rV=e4πε0e−2r/a0  ⟹  d2(rV)dr2=4a02e4πε0e−2r/a0r V = \frac{e}{4\pi\varepsilon_0} e^{-2r/a_0} \implies \frac{d^2(rV)}{dr^2} = \frac{4}{a_0^2} \frac{e}{4\pi\varepsilon_0} e^{-2r/a_0} ∇2V=eπε0a02e−2r/a0r  ⟹  ρ(r)=−ε0∇2V=−eπa02re−2r/a0\nabla^2 V = \frac{e}{\pi\varepsilon_0 a_0^2} \frac{e^{-2r/a_0}}{r} \implies \rho(r) = -\varepsilon_0 \nabla^2 V = -\frac{e}{\pi a_0^2 r} e^{-2r/a_0}


Problem 3: Steady-state conduction in a spherical shell

Shell of radii R1=0.10 mR_1 = 0.10 \text{ m} and R2=0.20 mR_2 = 0.20 \text{ m} has boundary temperatures T(R1)=100∘CT(R_1) = 100^\circ\text{C} and T(R2)=20∘CT(R_2) = 20^\circ\text{C}. Find T(r)T(r) and evaluate at midpoint r=0.15 mr = 0.15 \text{ m}.

Solution:

∇2T=0  ⟹  T(r)=−A/r+B\nabla^2 T = 0 \implies T(r) = -A/r + B −10A+B=100,−5A+B=20  ⟹  A=−16,B=−60-10A + B = 100, \quad -5A + B = 20 \implies A = -16, \quad B = -60 T(r)=16r−60T(r) = \frac{16}{r} - 60 T(0.15)=160.15−60≈46.67∘CT(0.15) = \frac{16}{0.15} - 60 \approx 46.67^\circ\text{C}