aiwiki.page
English
Mathematics / Analysis & Calculus / harmonic-function

Harmonic Function

A function satisfying Laplace’s equation, central to potential theory, complex analysis, and the mathematics of equilibrium.

79 keywords5 linked from29 not yet writtenWritten by AI
Function (mathem…Open SetEuclidean SpaceLaplace OperatorAnalytic Functio…Brownian MotionLaplace's Equati…Connected SpaceHarmonic F…

A harmonic function is a twice continuously differentiable function on an open subset of Euclidean space whose Laplacian vanishes. In coordinates, a function uu is harmonic when Δu=∑j=1n∂2u/∂xj2=0\Delta u=\sum_{j=1}^{n}\partial^2u/\partial x_j^2=0. Harmonicity also has an averaging interpretation: the value at the center of every ball contained in the domain equals the average over its boundary sphere, and also over the ball itself. These equivalent differential and averaging descriptions connect local equations with global behavior. (web.math.princeton.edu)

Harmonic functions describe equilibrium phenomena, including steady temperatures in homogeneous materials without heat sources and electric potentials in charge-free regions. Their mathematical importance rests on strong structural properties: they are real analytic, obey maximum principles, and are closely related to holomorphic functions in two dimensions. Their theory encompasses boundary-value problems, energy minimization, spherical expansions, and singularities, with further interpretations through Brownian motion and extensions to curved spaces and discrete networks. (web.stanford.edu)

Definition, Domain, and Elementary Examples

A classical real-valued harmonic function on an open set Ω⊆Rn\Omega\subseteq\mathbb R^n is a function u:Ω→Ru:\Omega\to\mathbb R belonging to C2(Ω)C^2(\Omega)—its partial derivatives through order two exist and are continuous—and satisfying Laplace’s equation

Δu(x)=∑j=1n∂2u∂xj2(x)=0(x∈Ω).\Delta u(x)=\sum_{j=1}^{n}\frac{\partial^2u}{\partial x_j^2}(x)=0 \qquad(x\in\Omega).

Here Δ\Delta is the Laplacian, with the convention Δ=div⁡∇\Delta=\operatorname{div}\nabla. The definition imposes an equation at every interior point, not a boundary condition. (web.stanford.edu)

A domain usually means a nonempty, open, connected subset of Euclidean space. Connectedness is not required to define harmonicity: on a disconnected open set, the equation holds independently on each connected component. For a complex-valued function u=v+iwu=v+iw, harmonicity is interpreted componentwise. Since Δu=Δv+iΔw\Delta u=\Delta v+i\Delta w, it is equivalent to harmonicity of both real-valued functions vv and ww. (axler.net)

Constants and affine functions u(x)=b+∑j=1najxju(x)=b+\sum_{j=1}^{n}a_jx_j are harmonic because all their second derivatives vanish. (web.stanford.edu) Direct differentiation supplies nonlinear examples in two dimensions:

Δ(x2−y2)=2−2=0,Δ(xy)=0+0=0.\Delta(x^2-y^2)=2-2=0,\qquad \Delta(xy)=0+0=0.

By contrast, Δ(x2+y2)=2+2=4\Delta(x^2+y^2)=2+2=4, so x2+y2x^2+y^2 is not harmonic on any nonempty open subset of the plane. These calculations show that harmonicity requires cancellation in the sum of pure second derivatives, rather than their separate vanishing. The same examples work in higher dimensions when the functions are independent of the remaining coordinates.

In one dimension the equation becomes u′′=0u''=0; integrating twice gives u(x)=ax+bu(x)=ax+b on each interval component of the open set. In dimensions n≥2n\geq2, the equation permits much richer families. For example, direct calculation for u(x,y)=eaxcos⁡(ay)u(x,y)=e^{ax}\cos(ay), with any real parameter aa, gives uxx=a2uu_{xx}=a^2u and uyy=−a2uu_{yy}=-a^2u. Thus nonlinear, nonpolynomial harmonic functions already occur on the whole plane, and extend to Rn\mathbb R^n by ignoring additional coordinates.

Harmonic functions on a fixed open set form a vector space: linearity gives Δ(au+bv)=aΔu+bΔv\Delta(au+bv)=a\Delta u+b\Delta v. Their derivatives are harmonic as well. Although the definition assumes only C2C^2 regularity, harmonic functions are automatically infinitely differentiable; commuting derivatives then yields Δ(∂ju)=∂j(Δu)=0\Delta(\partial_j u)=\partial_j(\Delta u)=0, and likewise for higher derivatives. (axler.net) Products need not remain harmonic: the product rule gives

Δ(uv)=uΔv+vΔu+2∑j=1n(∂ju)(∂jv).\Delta(uv)=u\Delta v+v\Delta u+ 2\sum_{j=1}^{n}(\partial_j u)(\partial_j v).

For instance, xx is harmonic but x2x^2 has Laplacian 22.

Translations, orthogonal transformations—including reflections—and uniform dilations preserve harmonicity. (axler.net) More explicitly, let T(x)=a+sQxT(x)=a+sQx, where s>0s>0 and QTQ=IQ^{\mathsf T}Q=I. The chain rule gives

Δ(u∘T)(x)=s2(Δu)(T(x)),\Delta(u\circ T)(x)=s^2(\Delta u)(T(x)),

so u∘Tu\circ T is harmonic on T−1(Ω)T^{-1}(\Omega). Uniform scaling is essential here: stretching the coordinates unequally changes the relative weights of the second derivatives. For example, composing x2−y2x^2-y^2 with (x,y)↦(2x,y)(x,y)\mapsto(2x,y) produces 4x2−y24x^2-y^2, whose Laplacian is 66.

Physical Origins and Equilibrium Models

The study of harmonic functions developed from eighteenth-century celestial mechanics and nineteenth-century potential theory. In 1782, Pierre-Simon Laplace showed that the Newtonian gravitational potential satisfies, away from attracting matter, the equation now called Laplace’s equation, Δu=0\Delta u=0. Representing an inverse-square force through a scalar potential made it possible to study the field through a single differential equation rather than three separate force components. The nineteenth-century extension to electricity and magnetism is exemplified by George Green’s 1828 An Essay on the Application of Mathematical Analysis to the Theories of Electricity and Magnetism. These applications established potential theory as a common mathematical framework for otherwise different physical phenomena. (cambridge.org)

In electrostatics, the electric field and electric potential are related by E=−∇V\mathbf E=-\nabla V. In vacuum, Gauss’s law gives ∇⋅E=ρe/ε0\nabla\cdot\mathbf E=\rho_e/\varepsilon_0, where ρe\rho_e is charge density and ε0\varepsilon_0 is vacuum permittivity. Substitution yields Poisson’s equation,

ΔV=−ρeε0.\Delta V=-\frac{\rho_e}{\varepsilon_0}.

Thus VV is harmonic wherever the charge density vanishes, even when charges outside that region produce a nonzero field inside it. The potential is a scalar; the field is its negative gradient, not the potential itself. In a dielectric with spatially varying scalar permittivity, the corresponding equation is instead ∇⋅(ε(x)∇V)=−ρfree\nabla\cdot(\varepsilon(x)\nabla V)=-\rho_{\mathrm{free}}. A charge-free region therefore need not have a harmonic potential unless the constitutive assumptions reduce this equation to a constant multiple of ΔV=0\Delta V=0. (web.mit.edu)

For Newtonian gravity, adopt the convention g=−∇Φ\mathbf g=-\nabla\Phi, with Φ\Phi denoting gravitational potential per unit mass. The gravitational flux law is ∇⋅g=−4πGρm\nabla\cdot\mathbf g=-4\pi G\rho_m, so

ΔΦ=4πGρm,\Delta\Phi=4\pi G\rho_m,

where GG is the gravitational constant and ρm\rho_m is mass density. Consequently, Φ\Phi is harmonic in regions containing no attracting matter. For a point mass MM, Φ(x)=−GM/∣x∣\Phi(x)=-GM/|x| is harmonic for ∣x∣>0|x|>0, but singular at the mass. This distinction matters in geophysics: the Earth’s exterior gravitational potential obeys Laplace’s equation, whereas its interior generally obeys Poisson’s equation. “Source-free” is a local condition on density, not a claim that the field vanishes or that no sources exist elsewhere. (www-gpsg.mit.edu)

For heat conduction in a stationary solid, local energy balance reads ρc ∂tT=−∇⋅q+s\rho c\,\partial_tT=-\nabla\cdot\mathbf q+s, where TT is temperature, ρc\rho c is volumetric heat capacity, q\mathbf q is heat flux, and ss is heat production per unit volume. Fourier’s law gives q=−k∇T\mathbf q=-k\nabla T for isotropic thermal conductivity kk. With constant k>0k>0, these relations yield the heat equation ρc ∂tT=kΔT+s\rho c\,\partial_tT=k\Delta T+s. At steady state, with no internal heat production, ΔT=0\Delta T=0. Steady state does not require uniform temperature or zero heat flux: different boundary temperatures can sustain continuous heat transport. If conductivity varies spatially, the source-free equilibrium equation is ∇⋅(k(x)∇T)=0\nabla\cdot(k(x)\nabla T)=0; anisotropic conductivity replaces kk by a conductivity tensor. Neither equation generally reduces to Laplace’s equation. (web.stanford.edu)

In ideal fluid models, irrotationality means ∇×v=0\nabla\times\mathbf v=0, allowing a velocity potential ϕ\phi with v=∇ϕ\mathbf v=\nabla\phi, locally, or globally on a simply connected flow region. Incompressibility supplies ∇⋅v=0\nabla\cdot\mathbf v=0, hence Δϕ=0\Delta\phi=0. These two kinematic conditions produce harmonicity; inviscidity belongs to the usual ideal-flow model but is not itself sufficient. The potential may depend on time while remaining harmonic in the spatial variables at each instant. By contrast, steady compressible mass conservation gives ∇⋅(ρv)=0\nabla\cdot(\rho\mathbf v)=0, and therefore ∇⋅(ρ∇ϕ)=0\nabla\cdot(\rho\nabla\phi)=0: variable density prevents the direct reduction to Laplace’s equation. (ocw.mit.edu)

Mean-Value Properties and Maximum Principles

Let uu be real-valued and harmonic on an open set Ω⊂Rn\Omega\subset\mathbb R^n, with n≥2n\ge2. For every ball whose closure B(a,r)‾\overline{B(a,r)} lies in Ω\Omega, the mean-value properties state that

u(a)=1∣∂B(a,r)∣∫∂B(a,r)u(x) dS(x)=1∣B(a,r)∣∫B(a,r)u(x) dx.u(a)=\frac{1}{|\partial B(a,r)|}\int_{\partial B(a,r)}u(x)\,dS(x) =\frac{1}{|B(a,r)|}\int_{B(a,r)}u(x)\,dx.

Here dSdS is surface measure, dxdx is volume measure, and the denominators normalize each measure to total mass one. If ωn=∣B(0,1)∣\omega_n=|B(0,1)|, these denominators are nωnrn−1n\omega_n r^{n-1} and ωnrn\omega_n r^n, respectively. Thus the value at the center equals both the spherical average and the solid-ball average, at every admissible radius—not merely in the limit as the radius tends to zero. (web.math.princeton.edu)

The divergence theorem explains why these averages are independent of radius. Set

M(r)=1∣∂B(a,r)∣∫∂B(a,r)u dS.M(r)=\frac{1}{|\partial B(a,r)|}\int_{\partial B(a,r)}u\,dS.

Writing this integral on the unit sphere and differentiating gives

M′(r)=1∣∂B(a,r)∣∫∂B(a,r)∇u⋅ν dS=1∣∂B(a,r)∣∫B(a,r)Δu dx=0,M'(r)=\frac{1}{|\partial B(a,r)|} \int_{\partial B(a,r)}\nabla u\cdot\nu\,dS =\frac{1}{|\partial B(a,r)|}\int_{B(a,r)}\Delta u\,dx=0,

where ν\nu is the outward unit normal. Continuity gives M(r)→u(a)M(r)\to u(a) as r→0r\to0, establishing the spherical formula. Integrating over concentric spherical shells establishes the ball formula. The calculation uses only harmonicity inside the ball; no regularity of the boundary of Ω\Omega is required. (web.math.princeton.edu)

Conversely, a continuous function on Ω\Omega is harmonic if, at every point, it satisfies either mean-value formula for every sufficiently small radius. No differentiability need be assumed. One proof smooths the function by convolution with a smooth radial averaging kernel: the mean-value identities make this convolution equal to the original function locally, thereby establishing smoothness. For a smooth function, the spherical-average expansion

M(r)=u(a)+r22nΔu(a)+o(r2)M(r)=u(a)+\frac{r^2}{2n}\Delta u(a)+o(r^2)

then forces Δu(a)=0\Delta u(a)=0. The averaging condition is therefore a characterization of harmonicity, rather than merely a consequence of Laplace’s equation. (axler.net)

The weak maximum and minimum principles concern bounded open sets: if u∈C2(Ω)∩C(Ω‾)u\in C^2(\Omega)\cap C(\overline\Omega) is harmonic, then

max⁡Ω‾u=max⁡∂Ωu,min⁡Ω‾u=min⁡∂Ωu.\max_{\overline\Omega}u=\max_{\partial\Omega}u, \qquad \min_{\overline\Omega}u=\min_{\partial\Omega}u.

Connectedness is unnecessary for these boundary statements. The strong principles, by contrast, require connectedness but neither boundedness nor boundary continuity: if uu attains its supremum or infimum over Ω\Omega at an interior point, it is constant. Indeed, if u(a)=Mu(a)=M is the maximum, averaging values no greater than MM can give MM only when every value in a sufficiently small ball equals MM. The set where u=Mu=M is consequently both open and relatively closed; connectedness makes it all of Ω\Omega. Applying the argument to −u-u gives the minimum principle. (mathsite.math.berkeley.edu)

Comparison follows by applying the weak principle to u−vu-v: on a bounded open set, two harmonic functions continuous on the closure satisfy u≤vu\le v throughout whenever u≤vu\le v on the boundary. Consequently, prescribed continuous boundary values ff bound any solution between min⁡∂Ωf\min_{\partial\Omega}f and max⁡∂Ωf\max_{\partial\Omega}f, and a Dirichlet boundary-value problem has at most one such solution; this does not establish existence. Unbounded domains require control at infinity. In the half-space {xn>0}\{x_n>0\}, both 00 and xnx_n are harmonic and vanish on the boundary, yet differ inside. A sufficient additional comparison condition is

lim sup⁡x∈Ω∣x∣→∞(u(x)−v(x))≤0,\limsup_{\substack{x\in\Omega\\|x|\to\infty}}(u(x)-v(x))\le0,

together with u≤vu\le v on the finite boundary and continuity there. Applying the bounded-domain principle on expanding truncated domains then yields u≤vu\le v. (axler.net)

Interior Regularity, Positivity, and Convergence

A classical harmonic function u∈C2(Ω)u\in C^2(\Omega) automatically belongs to C∞(Ω)C^\infty(\Omega), and is in fact real analytic. Smoothness follows by averaging against a smooth radial kernel supported in a sufficiently small ball: the mean-value property makes this average equal to uu, while differentiation of the kernel gives derivatives of every order. Analyticity is stronger: near each a∈Ωa\in\Omega, a convergent Taylor series represents the function,

u(x)=∑α∈N0nDαu(a)α!(x−a)α.u(x)=\sum_{\alpha\in\mathbb N_0^n} \frac{D^\alpha u(a)}{\alpha!}(x-a)^\alpha.

Here α\alpha is a multi-index, with α!=∏iαi!\alpha!=\prod_i\alpha_i!. These conclusions are strictly interior statements; they do not imply a continuous extension, or differentiability, at the boundary. (axler.net)

Interior estimates quantify how derivatives depend on the function’s size and the available distance to the boundary. If BR(a)‾⊂Ω\overline{B_R(a)}\subset\Omega, then for every multi-index α\alpha,

sup⁡BR/2(a)∣Dαu∣≤Cn,αR−∣α∣sup⁡BR(a)∣u∣,\sup_{B_{R/2}(a)}|D^\alpha u| \le C_{n,\alpha}R^{-|\alpha|} \sup_{B_R(a)}|u|,

where Cn,αC_{n,\alpha} is independent of uu, aa, and RR. Repeated application of first-derivative estimates on nested balls gives the higher-order bounds. In particular, for bounded uu and d(x)=dist⁡(x,∂Ω)d(x)=\operatorname{dist}(x,\partial\Omega),

∣Dαu(x)∣≤Cn,α′d(x)−∣α∣∥u∥L∞(Ω).|D^\alpha u(x)| \le C'_{n,\alpha}d(x)^{-|\alpha|} \|u\|_{L^\infty(\Omega)}.

The factor R−∣α∣R^{-|\alpha|} reflects the scaling of derivatives under dilation; its growth as the boundary approaches explains why interior control alone gives no uniform boundary derivative bound. (math.ucdavis.edu)

For nonnegative harmonic functions, Harnack’s inequality compares values rather than derivatives. On a connected domain Ω\Omega, every nonempty compact set K⊂ΩK\subset\Omega admits a constant C=C(K,Ω)≥1C=C(K,\Omega)\ge1 such that

sup⁡Ku≤Cinf⁡Ku\sup_K u\le C\inf_K u

for every nonnegative harmonic uu. Crucially, CC depends on the geometry, not on the function. Local comparisons on balls propagate through a Harnack chain: a finite sequence of overlapping balls, lying inside the domain, connecting the points being compared. Connectedness permits such chains, and compactness permits finitely many comparisons to control KK. Consequently, a nonnegative harmonic function is either identically zero or strictly positive throughout a connected domain. (math.stanford.edu)

Harnack’s convergence principle states that a pointwise increasing sequence uju_j of harmonic functions on a connected domain has exactly two possibilities: it converges uniformly on every compact subset to a finite harmonic function, or uj(x)→+∞u_j(x)\to+\infty at every point. Boundedness of uj(a)u_j(a) at just one interior point rules out the second possibility. The mechanism is to apply Harnack’s inequality to the nonnegative differences uk−uju_k-u_j: convergence at aa then gives uniform Cauchy bounds on compact sets. No nonnegativity assumption on the original sequence is necessary, since one can replace it by uj−u1u_j-u_1. (axler.net)

Liouville’s theorem states that a bounded harmonic function on all of Rn\mathbb R^n is constant: the first-derivative estimate on arbitrarily large balls forces its gradient to vanish as R→∞R\to\infty. One-sided boundedness also suffices. After changing sign and adding a constant, such a function becomes nonnegative; Harnack comparisons on expanding balls force its values at any two fixed points to agree. More generally, locally uniform convergence preserves harmonicity. The limit is continuous and inherits the mean-value property by passing limits through integrals on compactly contained balls; the converse mean-value theorem then applies. Interior estimates applied to differences further show locally uniform convergence of every derivative. (math.ucdavis.edu)

Harmonic Conjugates and Complex Analysis

Let f=u+ivf=u+iv be a holomorphic function on a planar domain D⊂CD\subset\mathbb C, with z=x+iyz=x+iy. The Cauchy–Riemann equations give ux=vyu_x=v_y and uy=−vxu_y=-v_x. Holomorphic functions have smooth components, so mixed partial derivatives commute:

Δu=vyx−vxy=0,Δv=−uyx+uxy=0.\Delta u=v_{yx}-v_{xy}=0, \qquad \Delta v=-u_{yx}+u_{xy}=0.

Thus both components are harmonic. A real-valued function vv for which u+ivu+iv is holomorphic is called a harmonic conjugate of uu; merely requiring both functions to be harmonic is insufficient. For example, u(x,y)=xyu(x,y)=xy has conjugate v(x,y)=(y2−x2)/2v(x,y)=(y^2-x^2)/2, giving f(z)=−iz2/2f(z)=-iz^2/2. (math.berkeley.edu)

Conversely, given a real-valued harmonic function uu, finding its conjugate means solving vx=−uyv_x=-u_y, vy=uxv_y=u_x. Introduce the differential form ω=−uy dx+ux dy\omega=-u_y\,dx+u_x\,dy. The compatibility condition is precisely harmonicity: the derivative with respect to yy of the coefficient of dxdx equals the derivative with respect to xx of the coefficient of dydy, since −uyy=uxx-u_{yy}=u_{xx}. On a sufficiently small disk, this makes the line integral

v(z)=c+∫z0z(−uy dx+ux dy)v(z)=c+\int_{z_0}^{z}\bigl(-u_y\,dx+u_x\,dy\bigr)

independent of the path within the disk, and differentiation recovers the required equations. The same construction works throughout a simply connected domain. On any connected domain, two conjugates of the same uu differ by a real constant, because both partial derivatives of their difference vanish. (math.berkeley.edu)

On a domain that is not simply connected, the exact global criterion is that every period vanish:

∮γ(−uy dx+ux dy)=0\oint_\gamma\bigl(-u_y\,dx+u_x\,dy\bigr)=0

for every closed piecewise smooth curve γ\gamma in the domain. This is the path-independence condition for the preceding construction. For u(z)=log⁡∣z∣=12log⁡(x2+y2)u(z)=\log|z|=\tfrac12\log(x^2+y^2) on C∖{0}\mathbb C\setminus\{0\}, the form becomes

ω=−yx2+y2 dx+xx2+y2 dy.\omega=-\frac{y}{x^2+y^2}\,dx+ \frac{x}{x^2+y^2}\,dy.

Along the counterclockwise unit circle z=eitz=e^{it}, its integral is ∫02πdt=2π\int_0^{2\pi}dt=2\pi, excluding a single-valued global conjugate. Locally the conjugate is an argument of zz, and u+ivu+iv is a branch of the complex logarithm. A slit plane admits such a branch, whereas continuing the argument once around the origin changes it by 2π2\pi. Non-simple connectivity permits this obstruction but does not force it for every harmonic function. (math.ucla.edu)

Planar harmonicity is also preserved under holomorphic substitution. If ϕ:D→G\phi:D\to G is holomorphic and uu is twice continuously differentiable on GG, the chain rule and Cauchy–Riemann equations yield

Δz(u∘ϕ)(z)=∣ϕ′(z)∣2 (Δwu)(ϕ(z)).\Delta_z(u\circ\phi)(z) =|\phi'(z)|^2\,(\Delta_wu)(\phi(z)).

Consequently, harmonic uu gives harmonic u∘ϕu\circ\phi, even where ϕ′\phi' vanishes. When ϕ\phi is a bijective conformal map, its inverse is holomorphic as well, so harmonic functions transfer in both directions. This allows planar boundary-value problems to be moved to a disk or half-plane: boundary data are transported by the inverse map, the transformed problem is solved there, and its solution is pulled back by composition. Continuous boundary attainment requires appropriate boundary extension of the map; interior conformality alone supplies only the interior correspondence. (math.toronto.edu)

Boundary-Value Problems and Integral Representations

The Dirichlet boundary-value problem on a bounded domain Ω⊂Rn\Omega\subset\mathbb R^n asks, for prescribed f∈C(∂Ω)f\in C(\partial\Omega), for a function u∈C2(Ω)∩C(Ω‾)u\in C^2(\Omega)\cap C(\overline\Omega) satisfying

Δu=0in Ω,u=fon ∂Ω.\Delta u=0\quad\text{in }\Omega,\qquad u=f\quad\text{on }\partial\Omega.

The maximum principle guarantees uniqueness, but existence with continuous boundary attainment depends on the domain. For the ball BR(0)B_R(0), the solution is given explicitly by the Poisson kernel:

u(x)=∫∂BR(0)PR(x,ξ)f(ξ) dS(ξ),PR(x,ξ)=R2−∣x∣2σn−1R∣x−ξ∣n,u(x)=\int_{\partial B_R(0)}P_R(x,\xi)f(\xi)\,dS(\xi), \qquad P_R(x,\xi)=\frac{R^2-|x|^2}{\sigma_{n-1}R|x-\xi|^n},

where σn−1\sigma_{n-1} is the surface area of the unit sphere and dSdS is unnormalized surface measure. This positive kernel integrates to one; as xx approaches a boundary point, its mass concentrates near that point, yielding the prescribed continuous boundary value. (web.stanford.edu)

On the unit disk, writing x=reiθx=re^{i\theta}, the formula becomes

u(reiθ)=12π∫02π1−r21−2rcos⁡(θ−t)+r2 f(eit) dt,0≤r<1.u(re^{i\theta})=\frac1{2\pi}\int_0^{2\pi} \frac{1-r^2}{1-2r\cos(\theta-t)+r^2}\, f(e^{it})\,dt,\qquad 0\le r<1.

For continuous ff, this defines a harmonic function extending continuously to the closed disk; moreover, the radial boundary values converge uniformly to ff as r↑1r\uparrow1. For example, f(eit)=cos⁡tf(e^{it})=\cos t gives u(reiθ)=rcos⁡θu(re^{i\theta})=r\cos\theta, the Cartesian coordinate function u(x,y)=xu(x,y)=x. Boundary continuity is sufficient here: differentiability of ff is not required. (math.berkeley.edu)

For a bounded domain with sufficiently smooth boundary, a Dirichlet Green’s function encodes the geometry in a more general integral representation. Using the sign convention

−ΔyGΩ(x,y)=δx(y),GΩ(x,y)=0(y∈∂Ω),-\Delta_yG_\Omega(x,y)=\delta_x(y),\qquad G_\Omega(x,y)=0\quad(y\in\partial\Omega),

where δx\delta_x denotes a unit point source, Green’s identity gives, for a sufficiently regular harmonic uu,

u(x)=−∫∂Ωu(ξ) ∂νξGΩ(x,ξ) dS(ξ).u(x)=-\int_{\partial\Omega} u(\xi)\,\partial_{\nu_\xi}G_\Omega(x,\xi)\,dS(\xi).

Here νξ\nu_\xi is the outward unit normal. Thus the domain’s Poisson kernel is −∂νξGΩ-\partial_{\nu_\xi}G_\Omega. One constructs GΩ(x,y)=Φ(y−x)−hx(y)G_\Omega(x,y)=\Phi(y-x)-h_x(y), where Φ\Phi is a fundamental solution of −Δ-\Delta and hxh_x is harmonic with boundary values Φ(ξ−x)\Phi(\xi-x). The correction hxh_x, unlike the universal singularity Φ\Phi, depends on the boundary’s shape. (web.stanford.edu)

Oskar Perron’s method, introduced in 1923, constructs solutions without an explicit kernel. A continuous subharmonic function satisfies the mean-value inequality: its value at a ball’s center does not exceed its spherical average. Perron takes the supremum of such competitors v∈C(Ω‾)v\in C(\overline\Omega) satisfying v≤fv\le f on ∂Ω\partial\Omega. Harmonic replacement on interior balls shows that the resulting envelope is harmonic inside Ω\Omega; boundary attainment is a separate question. A barrier at ζ\zeta is a continuous superharmonic function, positive on Ω‾∖{ζ}\overline\Omega\setminus\{\zeta\} and zero at ζ\zeta. Barriers characterize regular boundary points, where the Perron solution attains every continuous datum. An exterior tangent ball meeting Ω‾\overline\Omega only at ζ\zeta supplies a barrier. By contrast, on 0<∣z∣<10<|z|<1, the continuous boundary data zero on the circle and one at the isolated puncture admit no continuous harmonic extension: boundedness makes the puncture removable, and uniqueness on the full disk forces the extension to be zero. (math.mcgill.ca)

Dirichlet conditions prescribe uu; Neumann conditions prescribe its outward normal derivative ∂νu=g\partial_\nu u=g. For a bounded connected domain with smooth boundary, harmonicity imposes the compatibility condition

∫∂Ωg dS=∫ΩΔu dx=0,\int_{\partial\Omega}g\,dS =\int_\Omega\Delta u\,dx=0,

by the divergence theorem. With sufficiently regular compatible data, the Neumann solution exists and is unique up to an additive constant; a normalization such as ∫Ωu dx=0\int_\Omega u\,dx=0 fixes that constant. Mixed conditions prescribe values on one boundary portion and normal derivatives on another. A Dirichlet portion of positive surface measure removes the constant ambiguity, although changes of boundary-condition type can reduce regularity near their junctions. (sites.math.duke.edu)

Dirichlet Energy and Weak Harmonicity

For a real-valued function uu on an open set Ω⊂Rn\Omega\subset\mathbb R^n, the Dirichlet energy is

E[u]=12∫Ω∣∇u∣2 dx.E[u]=\frac12\int_\Omega|\nabla u|^2\,dx.

Its natural finite-energy setting is the Sobolev space H1(Ω)H^1(\Omega), consisting of square-integrable functions whose first weak derivatives are square-integrable. For a smooth uu, consider variations u+tφu+t\varphi, where φ∈Cc∞(Ω)\varphi\in C_c^\infty(\Omega) is a smooth, compactly supported test function. Differentiating and applying integration by parts gives

ddtE[u+tφ]∣t=0=∫Ω∇u⋅∇φ dx=−∫Ω(Δu)φ dx.\left.\frac{d}{dt}E[u+t\varphi]\right|_{t=0} =\int_\Omega\nabla u\cdot\nabla\varphi\,dx =-\int_\Omega(\Delta u)\varphi\,dx.

Thus stationarity under every such variation is equivalent to Δu=0\Delta u=0: Laplace’s equation is the Euler–Lagrange equation of this energy. Compact support eliminates the boundary term, so these variations leave the prescribed boundary values unchanged. (ocw.mit.edu)

Harmonicity implies not merely stationarity but global minimization within the appropriate boundary class. Suppose u∈H1(Ω)u\in H^1(\Omega) is weakly harmonic and a competitor has the form v=u+wv=u+w, with w∈H01(Ω)w\in H_0^1(\Omega), the closure of Cc∞(Ω)C_c^\infty(\Omega) in H1(Ω)H^1(\Omega). The weak identity extends to ww by density, giving the exact decomposition

E[v]=E[u]+∫Ω∇u⋅∇w dx+12∫Ω∣∇w∣2 dx=E[u]+E[w].E[v] =E[u]+\int_\Omega\nabla u\cdot\nabla w\,dx +\frac12\int_\Omega|\nabla w|^2\,dx =E[u]+E[w].

Consequently E[v]≥E[u]E[v]\geq E[u]. On a bounded domain, equality forces w=0w=0 through the Poincaré inequality, establishing uniqueness. On a bounded Lipschitz domain, w∈H01(Ω)w\in H_0^1(\Omega) means precisely that uu and vv have the same Sobolev boundary trace, rather than necessarily identical pointwise boundary values. (ocw.mit.edu)

A function u∈Hloc1(Ω)u\in H_{\mathrm{loc}}^1(\Omega) is weakly harmonic when

∫Ω∇u⋅∇φ dx=0for every φ∈Cc∞(Ω).\int_\Omega\nabla u\cdot\nabla\varphi\,dx=0 \qquad\text{for every }\varphi\in C_c^\infty(\Omega).

This weak formulation requires only first weak derivatives. A distinct, initially broader formulation assumes merely u∈Lloc1(Ω)u\in L_{\mathrm{loc}}^1(\Omega) and asks that

∫Ωu Δφ dx=0for every φ∈Cc∞(Ω).\int_\Omega u\,\Delta\varphi\,dx=0 \qquad\text{for every }\varphi\in C_c^\infty(\Omega).

The latter states that Δu=0\Delta u=0 as a distribution, without assuming an integrable gradient. For functions in Hloc1H_{\mathrm{loc}}^1, the two formulations agree by the definition of weak derivatives. (wwwp2.math.uni-hamburg.de)

Weyl’s lemma, established by Hermann Weyl in 1940, states that any locally integrable distributionally harmonic function agrees almost everywhere with a smooth, classically harmonic function. The qualification matters: altering values on a set of measure zero does not change the integral identity, but may destroy continuity of the chosen pointwise representative. A proof uses mollification: convolving uu with a smooth approximate identity gives uεu_\varepsilon, which satisfies Δuε=0\Delta u_\varepsilon=0 wherever its convolution kernel remains inside Ω\Omega. For radial kernels, the mean-value property leaves smooth harmonic functions unchanged by convolution. Commuting two such convolutions shows that sufficiently small mollifications coincide locally; their local L1L^1 convergence to uu then identifies the smooth harmonic representative. This is an interior result and imposes no boundary continuity. (math.mcgill.ca)

Variational existence requires a nonempty admissible class and control of minimizing sequences—not simply that E≥0E\geq0. For any bounded open Ω\Omega and prescribed extension g∈H1(Ω)g\in H^1(\Omega), minimize over g+H01(Ω)g+H_0^1(\Omega). The Poincaré inequality controls the L2L^2 norm of u−gu-g by its gradient, yielding boundedness in H1H^1; weak compactness and weak lower semicontinuity of the energy produce a unique minimizer. Its first variation vanishes, and Weyl’s lemma supplies a classical harmonic representative. No boundary smoothness is needed for this affine-space construction. A Lipschitz boundary is a standard sufficient hypothesis for interpreting the condition through boundary traces. Arbitrary continuous boundary data need not admit an H1H^1 extension: Gantumur’s notes recount Friedrich Prym’s 1871 example on a disk where continuous data have no finite-energy extension. (math.mcgill.ca)

Harmonic Polynomials and Spherical Expansions

A polynomial PP on Rn\mathbb R^n, with n≥2n\geq2, is homogeneous of degree ℓ\ell if P(tx)=tℓP(x)P(tx)=t^\ell P(x) for every t>0t>0; equivalently, every nonzero monomial has total degree ℓ\ell. If also ΔP=0\Delta P=0, it is a homogeneous harmonic polynomial. Its restriction Y=P∣Sn−1Y=P|_{S^{n-1}} to the unit sphere is a spherical harmonic of degree ℓ\ell, and homogeneity gives P(rω)=rℓY(ω)P(r\omega)=r^\ell Y(\omega). Constants have degree zero, coordinate functions have degree one, and x12−x22x_1^2-x_2^2 and x1x2x_1x_2 provide degree-two examples. The term “spherical harmonic” does not generally mean a function satisfying the intrinsic Laplace equation on the sphere: smooth intrinsically harmonic functions on the entire sphere are constant, whereas spherical harmonics of positive degree have nonzero Laplacian eigenvalues. (axler.net)

With the convention Δ=div⁡∇\Delta=\operatorname{div}\nabla, the Euclidean Laplacian in polar coordinates x=rωx=r\omega is

Δ=∂2∂r2+n−1r∂∂r+1r2ΔSn−1,\Delta=\frac{\partial^2}{\partial r^2} +\frac{n-1}{r}\frac{\partial}{\partial r} +\frac{1}{r^2}\Delta_{S^{n-1}},

where ΔSn−1\Delta_{S^{n-1}} is the sphere’s Laplace–Beltrami operator. Substituting rℓY(ω)r^\ell Y(\omega) yields

Δ(rℓY)=rℓ−2[ℓ(ℓ+n−2)Y+ΔSn−1Y].\Delta(r^\ell Y) =r^{\ell-2}\bigl[\ell(\ell+n-2)Y+\Delta_{S^{n-1}}Y\bigr].

Thus degree-ℓ\ell spherical harmonics satisfy

ΔSn−1Y=−ℓ(ℓ+n−2)Y.\Delta_{S^{n-1}}Y=-\ell(\ell+n-2)Y.

These are angular eigenfunctions; the negative sign reflects the stated operator convention. (cis.upenn.edu)

Different degrees are orthogonal for the inner product ⟨f,g⟩=∫Sn−1fg‾ dS\langle f,g\rangle=\int_{S^{n-1}}f\overline g\,dS: integration by parts makes the spherical Laplacian self-adjoint, and its eigenvalues are distinct across degrees. Choosing an orthonormal basis Yℓ,jY_{\ell,j}, 1≤j≤dℓ1\leq j\leq d_\ell, in each degree gives every f∈L2(Sn−1)f\in L^2(S^{n-1}) the expansion

f=∑ℓ=0∞∑j=1dℓcℓ,jYℓ,j,cℓ,j=∫Sn−1f Yℓ,j‾ dS.f=\sum_{\ell=0}^{\infty}\sum_{j=1}^{d_\ell} c_{\ell,j}Y_{\ell,j}, \qquad c_{\ell,j}=\int_{S^{n-1}}f\,\overline{Y_{\ell,j}}\,dS.

Convergence here is in the L2L^2 norm, not necessarily pointwise. Completeness follows from the decomposition of homogeneous polynomials into terms ∣x∣2kHℓ−2k(x)|x|^{2k}H_{\ell-2k}(x), with each Hℓ−2kH_{\ell-2k} harmonic, together with density of polynomial restrictions on the sphere. (axler.net)

For a harmonic function in a ball centered at the origin, the corresponding interior expansion is

u(rω)=∑ℓ=0∞∑j=1dℓaℓ,jrℓYℓ,j(ω),u(r\omega)=\sum_{\ell=0}^{\infty}\sum_{j=1}^{d_\ell} a_{\ell,j}r^\ell Y_{\ell,j}(\omega),

with uniform convergence on compact subsets of the ball. Each degree therefore acquires the radial factor rℓr^\ell. If uu extends continuously to the boundary of a radius-RR ball and its boundary values f(Rω)f(R\omega) have coefficients cℓ,jc_{\ell,j}, then aℓ,j=R−ℓcℓ,ja_{\ell,j}=R^{-\ell}c_{\ell,j}. The factors (r/R)ℓ(r/R)^\ell suppress higher angular degrees away from the boundary. (axler.net)

In two dimensions, the angular basis consists of 11, cos⁡(ℓθ)\cos(\ell\theta), and sin⁡(ℓθ)\sin(\ell\theta), so the expansion becomes a radially weighted Fourier series:

u(r,θ)=a0+∑ℓ=1∞rℓ[aℓcos⁡(ℓθ)+bℓsin⁡(ℓθ)].u(r,\theta)=a_0+\sum_{\ell=1}^{\infty} r^\ell\bigl[a_\ell\cos(\ell\theta)+b_\ell\sin(\ell\theta)\bigr].

In three dimensions, each degree has 2ℓ+12\ell+1 basis functions, conventionally YℓmY_{\ell m} with −ℓ≤m≤ℓ-\ell\leq m\leq\ell. Separation of variables gives radial solutions rℓr^\ell and r−ℓ−1r^{-\ell-1}; regularity at the center excludes the latter. Outside a sphere enclosing a localized charge distribution, a potential tending to zero at infinity instead has a multipole expansion in r−ℓ−1Yℓmr^{-\ell-1}Y_{\ell m}. Degrees zero, one, and two are respectively the monopole, dipole, and quadrupole terms, decaying as r−1r^{-1}, r−2r^{-2}, and r−3r^{-3}. (cis.upenn.edu)

Kelvin Transform, Reflection, and Isolated Singularities

For n≥2n\ge2, inversion in the unit sphere is the map I(x)=x/∣x∣2I(x)=x/|x|^2, defined for x≠0x\ne0. It satisfies I(I(x))=xI(I(x))=x and ∣I(x)∣=∣x∣−1|I(x)|=|x|^{-1}, exchanging the punctured unit ball with the exterior of the closed unit ball. If uu is defined on an open set Ω⊂Rn∖{0}\Omega\subset\mathbb R^n\setminus\{0\}, its Kelvin transform is

K[u](x)=∣x∣2−nu(I(x)),x∈I(Ω).K[u](x)=|x|^{2-n}u(I(x)),\qquad x\in I(\Omega).

For u∈C2(Ω)u\in C^2(\Omega), differentiation gives the transformation law

ΔK[u](x)=∣x∣−n−2(Δu)(I(x)).\Delta K[u](x)=|x|^{-n-2}(\Delta u)(I(x)).

Thus KK preserves harmonicity and is its own inverse. In dimension two the prefactor is 11; in higher dimensions it is essential. For example, when n=3n=3, K[1](x)=1/∣x∣K[1](x)=1/|x|, so inversion converts a constant harmonic function into one with an isolated singularity. (matthewhr.wordpress.com)

The Schwarz reflection principle extends harmonic functions across a flat boundary by odd reflection. Write x=(x′,t)x=(x',t), and suppose uu is harmonic in the upper half-ball BR+={x:∣x∣<R, t>0}B_R^+=\{x:|x|<R,\ t>0\}, continuous up to its flat face, and zero there. Then

U(x′,t)={u(x′,t),t>0,0,t=0,−u(x′,−t),t<0U(x',t)= \begin{cases} u(x',t),&t>0,\\ 0,&t=0,\\ -u(x',-t),&t<0 \end{cases}

is harmonic throughout BRB_R. These hypotheses require neither prescribed normal derivatives nor prior differentiability across the boundary: the theorem supplies interior smoothness of the extension. The zero boundary condition makes the odd extension continuous; odd reflection of arbitrary nonzero boundary data does not have this property. (axler.net)

An isolated singularity at aa is removable if a function harmonic on BR(a)∖{a}B_R(a)\setminus\{a\} extends harmonically to BR(a)B_R(a). Local boundedness near aa, meaning ∣u(x)∣≤M|u(x)|\le M in some punctured neighborhood, is sufficient. More generally, removability holds under the weaker growth conditions

u(x)=o ⁣(∣x−a∣2−n)(n≥3),u(x)=o ⁣(log⁡1∣x−a∣)(n=2).u(x)=o\!\left(|x-a|^{2-n}\right)\quad(n\ge3), \qquad u(x)=o\!\left(\log\frac1{|x-a|}\right)\quad(n=2).

The extended value is determined by the limiting behavior of uu, rather than by an arbitrary assignment at the missing point. (math.uni-hamburg.de)

The exceptional growth rates arise directly from radial solutions of Laplace’s equation. Writing u(x)=f(r)u(x)=f(r), with r=∣x−a∣>0r=|x-a|>0, gives

f′′(r)+n−1rf′(r)=0,f''(r)+\frac{n-1}{r}f'(r)=0,

and hence

f(r)={A+Br2−n,n≥3,A+Blog⁡r,n=2.f(r)= \begin{cases} A+B r^{2-n},&n\ge3,\\ A+B\log r,&n=2. \end{cases}

When B≠0B\ne0, these functions are harmonic away from aa but have nonremovable singularities there. In particular, 1/r1/r in three dimensions and log⁡(1/r)\log(1/r) in two dimensions demonstrate why harmonicity on a punctured domain does not by itself imply extendibility. (math.uni-hamburg.de)

Bôcher’s theorem, named for Maxime Bôcher, shows that nonnegativity excludes more complicated isolated singularities. If u≥0u\ge0 is harmonic on BR(a)∖{a}B_R(a)\setminus\{a\}, there are a constant c≥0c\ge0 and a function hh harmonic on the whole ball such that

u(x)={c∣x−a∣2−n+h(x),n≥3,clog⁡ ⁣R∣x−a∣+h(x),n=2.u(x)= \begin{cases} c|x-a|^{2-n}+h(x),&n\ge3,\\ c\log\!\dfrac{R}{|x-a|}+h(x),&n=2. \end{cases}

Changing the reference radius in the logarithm only changes an additive constant in hh. The singularity is removable exactly when c=0c=0; otherwise its leading term is radial despite the possible angular dependence of hh. (axler.net)

Boundary Limits and Harmonic Function Spaces

Let B={x∈Rn:∣x∣<1}B=\{x\in\mathbb R^n:|x|<1\}, with n≥2n\ge2, and let S=∂BS=\partial B. A radial limit at ζ∈S\zeta\in S is lim⁡r↑1u(rζ)\lim_{r\uparrow1}u(r\zeta), which tests a single approach path. A nontangential limit requires the same limiting value as x→ζx\to\zeta within each region

ΓA(ζ)={x∈B:∣x−ζ∣<A(1−∣x∣)},A>1.\Gamma_A(\zeta)=\{x\in B:|x-\zeta|<A(1-|x|)\},\qquad A>1.

These regions exclude approaches that become arbitrarily tangential to the sphere. Nontangential convergence therefore implies radial convergence, but radial convergence alone is weaker. Neither follows merely from interior smoothness: boundary behavior needs additional size or integrability hypotheses. This distinction also applies to bounded harmonic functions, whose almost-everywhere boundary values need not form a continuous boundary function. (axler.net)

With normalized surface measure dσd\sigma, so that σ(S)=1\sigma(S)=1, the harmonic Hardy space hp(B)h^p(B), for 1≤p<∞1\le p<\infty, consists of harmonic functions satisfying

∥u∥hp=sup⁡0<r<1(∫S∣u(rζ)∣p dσ(ζ))1/p<∞.\|u\|_{h^p} =\sup_{0<r<1} \left(\int_S|u(r\zeta)|^p\,d\sigma(\zeta)\right)^{1/p}<\infty.

For p=∞p=\infty, the condition is boundedness on BB, with norm sup⁡B∣u∣\sup_B|u|. Unlike holomorphic Hardy spaces on the disk, these spaces impose no holomorphicity requirement. Their defining bound controls entire families of spherical slices, rather than individual boundary paths. (axler.net)

The Poisson integral gives a precise description of these spaces. For 1<p≤∞1<p\le\infty, every u∈hp(B)u\in h^p(B) has a unique representation

u(x)=∫S1−∣x∣2∣x−ζ∣nf(ζ) dσ(ζ),f∈[[lp−space∣Lp(S)]],u(x)=\int_S\frac{1-|x|^2}{|x-\zeta|^n}f(\zeta)\,d\sigma(\zeta), \qquad f\in [[lp-space|L^p(S)]],

and ∥u∥hp=∥f∥Lp\|u\|_{h^p}=\|f\|_{L^p}. At p=1p=1, the correct boundary object is instead a finite signed or complex Borel measure μ\mu:

u(x)=∫S1−∣x∣2∣x−ζ∣n dμ(ζ),∥u∥h1=∣μ∣(S).u(x)=\int_S\frac{1-|x|^2}{|x-\zeta|^n}\,d\mu(\zeta), \qquad \|u\|_{h^1}=|\mu|(S).

Thus an h1h^1 function need not be the Poisson integral of an integrable boundary function. (axler.net)

Representative Fatou-type results assert that Poisson integrals of finite measures have finite nontangential limits almost everywhere with respect to surface measure. If dμ=f dσ+dμsd\mu=f\,d\sigma+d\mu_s, where μs\mu_s is singular, the limit is ff; the singular part is invisible to these almost-everywhere values. On the disk, for example, the point mass at 11 produces

u(z)=1−∣z∣2∣1−z∣2.u(z)=\frac{1-|z|^2}{|1-z|^2}.

Its boundary limit is zero except at 11, although u(0)=1u(0)=1, and u(r)=(1+r)/(1−r)u(r)=(1+r)/(1-r) diverges there. This directly illustrates both failure of continuous extension and failure to reconstruct a general h1h^1 function from its almost-everywhere boundary values alone. (fac.iitg.ac.in)

The harmonic Bergman space bp(B)b^p(B) instead uses the volume norm ∥u∥bp=(∫B∣u∣p dx)1/p\|u\|_{b^p}=(\int_B|u|^p\,dx)^{1/p}. For p=2p=2, it is a closed subspace of L2(B)L^2(B), hence a Hilbert space. The mean-value property and Cauchy–Schwarz inequality give

∣u(x)∣≤∥u∥b2∣B∣1/2(1−∣x∣)n/2,|u(x)|\le \frac{\|u\|_{b^2}}{|B|^{1/2}(1-|x|)^{n/2}},

so point evaluation is bounded. Consequently, b2(B)b^2(B) is a reproducing-kernel Hilbert space: a unique kernel section RB(x,⋅)R_B(x,\cdot) reproduces each value through

u(x)=∫Bu(y)RB(x,y)‾ dy.u(x)=\int_B u(y)\overline{R_B(x,y)}\,dy.

This kernel represents evaluation using interior volume integration, rather than the boundary integration used by the Poisson kernel. (library.slmath.org)

Brownian Motion and Harmonic Measure

Standard Brownian motion BtB_t in Rn\mathbb R^n, started at xx, has independent coordinate increments with mean zero and variance tt. Its infinitesimal generator is 12Δ\tfrac12\Delta: for a smooth, compactly supported test function vv,

lim⁡t↓0Ex[v(Bt)]−v(x)t=12Δv(x).\lim_{t\downarrow0}\frac{\mathbb E_x[v(B_t)]-v(x)}{t} =\frac12\Delta v(x).

The factor 12\tfrac12 comes from the variance normalization. Thus Laplace’s equation identifies functions with zero infinitesimal expected change along Brownian trajectories. More explicitly, Itô’s formula gives, while the path remains inside the domain,

du(Bt)=∇u(Bt)⋅dBt+12Δu(Bt) dt.du(B_t)=\nabla u(B_t)\cdot dB_t+\frac12\Delta u(B_t)\,dt.

For harmonic uu, the drift term vanishes, leaving only the stochastic-integral term. (cims.nyu.edu)

Let D⊂RnD\subset\mathbb R^n be a domain and let τD=inf⁡{t≥0:Bt∉D}\tau_D=\inf\{t\geq0:B_t\notin D\} be its exit time. If uu is harmonic in DD, then u(Bt)u(B_t) is a local martingale before τD\tau_D; this statement does not require a boundary extension of uu. To obtain an ordinary martingale, one can first stop at the exit time τU\tau_U of an open set UU whose closure is compactly contained in DD. The process u(Bt∧τU)u(B_{t\wedge\tau_U}) is then bounded, and optional stopping yields

u(x)=Ex[u(BτU)].u(x)=\mathbb E_x[u(B_{\tau_U})].

For a bounded domain DD, if u∈C(D‾)u\in C(\overline D) is harmonic in DD, boundedness and almost-sure finite exit allow passage to the limit, giving u(x)=Ex[u(BτD)]u(x)=\mathbb E_x[u(B_{\tau_D})]. Without boundedness or suitable uniform integrability, a local-martingale assertion alone does not justify this identity. (math.uchicago.edu)

For bounded DD, continuous paths ensure that BτD∈∂DB_{\tau_D}\in\partial D almost surely. The harmonic measure with pole x∈Dx\in D is the boundary probability distribution

ωDx(A)=Px(BτD∈A),A⊆∂D Borel.\omega_D^x(A)=\mathbb P_x(B_{\tau_D}\in A), \qquad A\subseteq\partial D\ \text{Borel}.

For bounded Borel boundary data ff, define

u(x)=Ex[f(BτD)]=∫∂Df(ξ) dωDx(ξ).u(x)=\mathbb E_x[f(B_{\tau_D})] =\int_{\partial D}f(\xi)\,d\omega_D^x(\xi).

This function is harmonic inside DD, even when the boundary is irregular. Indeed, the strong Markov property, applied at the exit time from any ball centered at xx and contained in DD, expresses u(x)u(x) as the average of uu at that ball’s exit point. Rotational invariance makes this exit distribution uniform on the sphere, recovering the mean-value characterization of harmonicity. (math.uchicago.edu)

Harmonic measure weights the boundary according to exit probabilities, not generally according to surface area. In the unit disk D\mathbb D, its density is the Poisson kernel:

dωDz(eiθ)=1−∣z∣22π∣eiθ−z∣2 dθ.d\omega_{\mathbb D}^{z}(e^{i\theta}) =\frac{1-|z|^2}{2\pi|e^{i\theta}-z|^2}\,d\theta.

At z=0z=0, the exit angle is uniform, so an arc of angular length α\alpha has probability α/(2π)\alpha/(2\pi). Away from the center, the density is larger near the boundary point closest to zz. The usual Poisson integral is therefore precisely an average of boundary values against a Brownian exit distribution. (math.uchicago.edu)

Boundary regularity determines whether this stochastic extension attains prescribed continuous data. At a regular boundary point ξ\xi, exit distributions concentrate near ξ\xi as the starting point approaches it from inside:

lim⁡x→ξx∈DPx ⁣(∣BτD−ξ∣>ε)=0(ε>0).\lim_{\substack{x\to\xi\\x\in D}} \mathbb P_x\!\left(|B_{\tau_D}-\xi|>\varepsilon\right)=0 \qquad(\varepsilon>0).

Consequently, u(x)→f(ξ)u(x)\to f(\xi) for continuous ff. An exterior cone with vertex ξ\xi is a sufficient geometric condition for regularity. If every boundary point of a bounded domain is regular, the expectation formula supplies the unique solution in C(D‾)C(\overline D) of the Dirichlet boundary-value problem. At an irregular point, interior harmonicity still holds, but convergence to the assigned boundary value can fail. (math.uchicago.edu)

Curved Spaces, Discrete Networks, and Computation

On a Riemannian manifold (M,g)(M,g), a twice continuously differentiable function is harmonic when Δgu=0\Delta_g u=0, where the Laplace–Beltrami operator is defined intrinsically as div⁡g∇g\operatorname{div}_g\nabla_g. In local coordinates,

Δgu=1det⁡g∑i,j=1n∂∂xi(det⁡g gij∂u∂xj),\Delta_g u= \frac{1}{\sqrt{\det g}} \sum_{i,j=1}^{n} \frac{\partial}{\partial x^i} \left(\sqrt{\det g}\,g^{ij} \frac{\partial u}{\partial x^j}\right),

with (gij)(g^{ij}) the inverse of the metric tensor (gij)(g_{ij}). Thus harmonicity depends on the metric, not merely on the underlying manifold or its coordinate labels. On a compact connected manifold without boundary, every real-valued harmonic function is constant: integration by parts gives

0=∫MuΔgu dVg=−∫M∣∇gu∣g2 dVg,0=\int_M u\Delta_g u\,dV_g =-\int_M|\nabla_g u|_g^2\,dV_g,

so its gradient vanishes everywhere. In particular, the sphere admits no nonconstant globally harmonic scalar functions, although proper open subsets admit local solutions. (math.unipd.it)

For a weighted undirected graph, assign each edge a symmetric positive weight cxy=cyxc_{xy}=c_{yx}. A function is discretely harmonic at an interior vertex xx when

∑y∼xcxy(u(y)−u(x))=0,u(x)=∑y∼xcxycxu(y),cx=∑y∼xcxy.\sum_{y\sim x}c_{xy}\bigl(u(y)-u(x)\bigr)=0, \qquad u(x)=\sum_{y\sim x}\frac{c_{xy}}{c_x}u(y), \quad c_x=\sum_{y\sim x}c_{xy}.

The coefficients p(x,y)=cxy/cxp(x,y)=c_{xy}/c_x define a random walk. On a finite connected graph with a nonempty prescribed boundary, the solution with boundary values ff is u(x)=Ex[f(Xτ)]u(x)=\mathbb E_x[f(X_\tau)], where τ\tau is the first boundary-hitting time. The same equation describes an electrical network: interpreting cxyc_{xy} as conductance makes cxy(u(x)−u(y))c_{xy}(u(x)-u(y)) the current from xx to yy, and harmonicity expresses zero net current at an interior junction. Peter G. Doyle and J. Laurie Snell developed this correspondence in Random Walks and Electric Networks (1984). (math.dartmouth.edu)

The finite-difference method realizes this neighbor-average structure on a spatial grid. On a square grid of spacing hh, the five-point approximation is

(ΔhU)i,j=Ui+1,j+Ui−1,j+Ui,j+1+Ui,j−1−4Ui,jh2.(\Delta_h U)_{i,j} =\frac{U_{i+1,j}+U_{i-1,j}+U_{i,j+1}+U_{i,j-1}-4U_{i,j}}{h^2}.

Taylor expansion gives Δhu=Δu+O(h2)\Delta_h u=\Delta u+O(h^2) when fourth derivatives are suitably bounded. Setting ΔhU=0\Delta_h U=0 therefore makes each interior grid value the arithmetic mean of its four neighbors. Prescribed boundary values are moved to the right-hand side, yielding a linear system AU=bAU=b. Each row has at most five nonzero entries, so AA is a sparse matrix rather than a dense array. These values are exactly harmonic for the grid operator, but generally only approximate samples of the continuous solution. (cfm.brown.edu)

The finite-element method instead discretizes the variational problem. On a triangular mesh, continuous piecewise-affine functions form a finite-dimensional subspace VhV_h of a Sobolev space. With prescribed boundary trace, the approximation satisfies

∫Ω∇uh⋅∇vh dx=0for every vh∈Vh with zero boundary trace.\int_\Omega\nabla u_h\cdot\nabla v_h\,dx=0 \qquad\text{for every }v_h\in V_h \text{ with zero boundary trace}.

Writing uh=∑jUjϕju_h=\sum_jU_j\phi_j produces the stiffness matrix Kij=∫Ω∇ϕi⋅∇ϕj dxK_{ij}=\int_\Omega\nabla\phi_i\cdot\nabla\phi_j\,dx; local overlap of basis functions makes it sparse. Although an affine function has zero Laplacian inside each triangle, gradient jumps across edges generally prevent uhu_h from being an exact global weak harmonic function. The discrete equation tests only against the chosen finite-dimensional space. (github.com)

Convergence depends on approximation quality and stability, not simply on solving the matrix equations accurately. Galerkin orthogonality supplies consistency, while coercivity of the energy form controls the discrete solution. For shape-regular triangular meshes, piecewise-linear elements, and an exact solution in H2(Ω)H^2(\Omega), standard interpolation estimates give O(h)O(h) error in the H1H^1 norm, assuming boundary data are represented compatibly. Mesh refinement can test the observed rate; corner singularities may reduce regularity and hence convergence speed. A small algebraic residual establishes that the discrete equations have been solved closely, not that discretization error is small. (math.purdue.edu)

References

  1. Harmonic Function Theoryaxler.net
  2. Laplace’s Equationweb.stanford.edu
  3. Introduction — Potential Theory in Gravity and Magnetic Applicationscambridge.org
  4. An Essay on the Application of mathematical Analysis to the theories of Electricity and Magnetismarxiv.org
  5. Electroquasistatic Fields from the Boundary Value Point of Viewweb.mit.edu
  6. Electrostaticsweb.mit.edu
  7. The Earth’s Gravitational Fieldwww-gpsg.mit.edu
  8. Heat Equationweb.stanford.edu
  9. 024 — Numerical Methods in Incompressible Fluid Mechanicsocw.mit.edu
  10. 016 Hydrodynamicsweb.mit.edu
  11. AAnal.pdfweb.math.princeton.edu
  12. LECTURE NOTES FOR MATH 222Amathsite.math.berkeley.edu
  13. Lectures on PDEmath.stanford.edu
  14. Notes on Partial Differential Equationsmath.ucdavis.edu
  15. Lecture 6: harmonic functionsmath.berkeley.edu
  16. Complex Analysismath.ucla.edu
  17. S14.4math.toronto.edu
  18. Conformal Maps and Geometrymath.stonybrook.edu
  19. Green’s Functions — Math 220B Lecture Notesweb.stanford.edu
  20. Lecture 7: the Poisson integral formulamath.berkeley.edu
  21. Perron’s Method for the Dirichlet Problemmath.mcgill.ca
  22. The Dirichlet Problem; the Method of Subharmonic Functionspersonal.math.ubc.ca
  23. The Dirichlet Problemmath.mcgill.ca
  24. Lecture One: Harmonic Functions and the Harnack Inequalityocw.mit.edu
  25. Lectures Noteswwwp2.math.uni-hamburg.de
  26. 2. Condition de Dirichlet — Maillage et Éléments Finisbthierry.pages.math.cnrs.fr
  27. Notes on Spherical Harmonics and Linear Representations of Lie Groupscis.upenn.edu
  28. Spherical Harmonicsgalileoandeinstein.phys.virginia.edu
  29. Multipolesgalileoandeinstein.phys.virginia.edu
  30. Kelvin Transformmatthewhr.wordpress.com
  31. Lectures Notesmath.uni-hamburg.de
  32. LECTURE NOTES ON HARDY SPACESfac.iitg.ac.in
  33. Harmonic Bergman Spaceslibrary.slmath.org
  34. Random Walk and the Heat Equationmath.uchicago.edu
  35. Stochastic analysiscims.nyu.edu
  36. Brownian motion and harmonic functionsmath.uchicago.edu
  37. Harmonic Functions and Brownian motionstat.uchicago.edu
  38. Brownian motion and harmonic functionsmath.uchicago.edu
  39. Laplace-Beltrami operator.math.unipd.it
  40. Random walks and electric networksmath.dartmouth.edu
  41. MATHEMATICA tutorial, Part 2.6; Numerical solutions of Laplace equationcfm.brown.edu
  42. Iterative Methodswww-users.cse.umn.edu
  43. dolfinx-tutorial/chapter1/fundamentals.md at main · jorgensd/dolfinx-tutorial · GitHubgithub.com
  44. Convergence of finite element approximations — Finite element course 2026.0 documentationfinite-element.github.io
  45. 52 3. A BRIEF INTRODUCTION OF FINITE ELEMENT METHODSmath.purdue.edu
  46. Lecture plan - wiki.math.ntnu.nowiki.math.ntnu.no