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Exterior waves, absorbing boundaries and PML

1 · Prerequisites

2 · Summary

The exterior model and angular, radial-flux and outgoing-mode foundations are placed on boundary-integral-equations-and-galerkin-bem, retaining their original item identifiers. This page uses them for the spherical-obstacle and truncation results below.

This page fixes the time factor e−iωt and proves the sound-soft exterior Helmholtz results for a centered spherical obstacle with smooth boundary data. Spherical harmonic projections reduce the exterior equation to radial modes; the outgoing spherical Hankel mode gives both the exact modal Dirichlet-to-Neumann (DtN) map and an exact variational truncation on a concentric annulus. The local impedance condition is compared with that exact map through its plane-wave and spherical-mode reflection coefficients.

The PML branch is Cartesian, homogeneous, and modewise. It proves exact matching at the interface and attenuation for propagating modes whose normal wavenumber stays bounded below. The finite layer calculation gives its exact reflected amplitude for a Dirichlet termination.

The two diagrams fix the geometric and sign conventions used in the formulas. The concentric curves denote the obstacle boundary Sa and artificial boundary SR, with 0<a<R; the PML coordinate begins at x=0, where its stretch is the identity.

\begin{tikzpicture}[scale=1.0]
  \draw[thick] (0,0) circle (0.75);
  \draw[thick,dashed] (0,0) circle (2.0);
  \fill (0,0) circle (1.4pt);
  \draw[->] (0,0) -- (0.75,0) node[midway,below] {$a$};
  \draw[->] (0,0) -- (2.0,0) node[midway,below] {$R$};
  \node at (0,0.25) {$B_a$};
  \node at (0,1.15) {$a<r<R$};
  \node at (0,2.25) {$S_R$};
  \draw[->,thick] (2.15,0.55) -- (2.75,0.55);
  \node[right] at (2.75,0.55) {outgoing};
\end{tikzpicture}
\begin{tikzpicture}[x=1.0cm,y=1.0cm]
  \draw[thick] (-2,0) -- (0,0);
  \draw[thick,fill=blue!8] (0,-0.8) rectangle (2.4,0.8);
  \draw[thick,dashed] (2.4,-0.8) -- (2.4,0.8);
  \draw[->,thick] (-1.8,0.25) -- (0,0.25);
  \draw[->,thick] (0,0.25) -- (1.8,0.25);
  \draw[->] (0,-0.55) -- (1.0,-0.55) node[midway,below] {$x$};
  \draw[->] (0,-0.55) -- (0,0.2) node[midway,left] {$y$};
  \node at (-1.0,0.65) {physical};
  \node at (1.2,0.65) {PML};
  \node[below] at (0,-0.8) {$x=0,\ X(0)=0$};
  \node[below] at (2.4,-0.8) {$x=L$};
\end{tikzpicture}

The arrows indicate an outgoing mode across the interface. In the PML strip the analytic coordinate is X(x)=x+iS(x), so the mode amplitude is multiplied by e−qS(x) only for a real positive normal wavenumber q. The proofs do not use either drawing.

3 · Logical flowchart

4 · Definitions, theorems and proofs

DefinitionDefinition: Literature-sourcedProof: Not applicablejudge pass (gpt-6-luna)Open item page →

Cartesian complex-stretch PML for a homogeneous Helmholtz mode

Definition

Let k>0, x∈R be the Cartesian normal coordinate, and y∈R2 the tangential coordinate. Let σ be nonnegative, continuous, piecewise C1, and zero for x≤0. Define S(x)=∫0xσ(t) dt,X(x)=x+iS(x),s(x)=X′(x)=1+iσ(x). The pulled-back constant-coefficient Helmholtz operator in the layer is 1s(x)∂x(1s(x)∂x)+Δy+k2. This definition concerns the homogeneous Cartesian branch only; it makes no claim for heterogeneous media, curved stretches, grazing or evanescent uniform attenuation, discretizations, or finite-element convergence.

DefinitionDefinition: Literature-sourcedProof: Not applicablejudge pass (gpt-6-luna)Open item page →

First-order local impedance condition at an artificial plane

Definition

Use the outgoing time convention e−iωt. On an artificial boundary with outward unit normal n, the first-order local impedance condition is ∂nu−iku=0. For the plane x=R with n=+ex, this is ∂xu−iku=0. It is the exact outgoing relation at normal incidence and an approximation for oblique propagating modes; no exactness or uniform small-reflection claim at grazing incidence is part of this definition.

TheoremStatement: Literature-sourcedProof: AI-adaptedprecheck passjudge pass (gpt-6-luna)Open item page →

Perfect matching and attenuation for non-grazing propagating modes

Statement

Let k>0, η∈R2 satisfy ∣η∣<k, and let q=k2−∣η∣2>0 be the outgoing normal branch. In the stretch of Cartesian complex-stretch PML for a homogeneous Helmholtz mode, u(x,y)=eiqX(x)+iη⋅y solves the pulled-back Helmholtz equation. At x=0, its value and normal flux (1/s)∂xu agree with those of the physical mode eiqx+iη⋅y. Its modulus is e−qS(x). If a family of modes satisfies q≥q0>0, then ∣u(x,y)∣≤e−q0S(x) uniformly; whenever S(x)≥σ0x for some σ0>0, this is at most e−q0σ0x. No uniform bound is asserted as q↓0.

Facts & Assumptions

Given: The constant-coefficient Cartesian operator and stretch data in [F1].

[F1]

Cartesian complex-stretch PML for a homogeneous Helmholtz mode: X=x+iS, s=X′=1+iσ, and the operator is s−1∂x(s−1∂x)+Δy+k2.

Proof

Given: k>0, ∣η∣<k, q=k2−∣η∣2, and [F1].

1.1givenF1algebra

For the stated mode, ∂xu=iqs(x)u, so s−1∂xu=iqu and s−1∂x(s−1∂xu)=s−1∂x(iqu)=−q2u. Also Δyu=−∣η∣2u. Since q2+∣η∣2=k2, substitution into [F1] gives zero.

2.1F1step 1.1algebra∎

At x=0, S(0)=0 and σ(0)=0 by continuity and the definition, so X(0)=0, s(0)=1, and the stretched mode and its normal flux equal eiη⋅y and iqeiη⋅y, respectively, exactly as in the physical outgoing mode. Since ∣eiq(x+iS)+iη⋅y∣=e−qS, the bounds follow from q≥q0 and, when assumed, S(x)≥σ0x. As q↓0, the attenuation bound tends to one, so this proof gives no uniform grazing decay.

LemmaStatement: Literature-sourcedProof: AI-adaptedprecheck passjudge pass (gpt-6-luna)Open item page →

Spherical Hankel modulus and uniform radial bounds

Statement

For integers ℓ≥0 and real z>0, write hℓ=hℓ(1) using Spherical Bessel and outgoing Hankel function conventions. Then ∣hℓ(z)∣2=∑m=0ℓSℓmz−2m−2,Sℓm=(2m)!(ℓ+m)!4m(m!)2(ℓ−m)!. Consequently ∣hℓ(z)∣ is nonincreasing in z, ∣hℓ−1(z)∣≤∣hℓ(z)∣ for ℓ≥1, and ∣hℓ′(z)∣≤(1+(ℓ+1)/z)∣hℓ(z)∣. For every fixed z0>0 and all z≥z0, ∣z(hℓ′(z)−ihℓ(z))∣∣hℓ(z0)∣≤(ℓ+1)e2z0.

Facts & Assumptions

Given: The finite-derivative outgoing Hankel convention and its radial recurrences.

[F1]

Spherical Bessel and outgoing Hankel function conventions: hℓ=(−z)ℓ(z−1d/dz)ℓ(−ieiz/z).

[F2]

Spherical Bessel and outgoing Hankel recurrences solve the radial Helmholtz equation: hℓ+1=ℓhℓ/z−hℓ′ and hℓ′=hℓ−1−(ℓ+1)hℓ/z for ℓ≥1.

Proof

Given: Integer ℓ≥0, real z>0, and [F1]–[F2].

1.1F1F2algebra

Direct differentiation of h0=−ieiz/z gives the finite expression hℓ(z)=(−i)ℓ+1eiz∑m=0ℓimAℓmz−m−1,Aℓm=(ℓ+m)!m!(ℓ−m)!2m. Indeed it holds at ℓ=0; substituting this expression in hℓ+1=ℓhℓ/z−hℓ′ gives Aℓ+1,m=Aℓm+(ℓ+m)Aℓ,m−1 (out-of-range coefficients are zero), and the displayed factorial formula satisfies that recurrence and the m=0 base.

2.1F1F2step 1.1algebra

Let Fℓ=∣hℓ∣2. The radial recurrence gives hℓ+1=(2ℓ+1)hℓ/z−hℓ−1. Also Fℓ′=2Re⁡(hˉℓhℓ−1)−2(ℓ+1)Fℓ/z by [F2]. Expanding the squared modulus and eliminating the real cross term yields Fℓ+1=Fℓ−1−(2ℓ+1)Fℓ′/z−(2ℓ+1)Fℓ/z2. From F0=z−2 and F1=z−2+z−4, coefficient comparison yields Sℓ+1,0=Sℓ−1,0=1 and, for 1≤q≤ℓ, Sℓ+1,q=Sℓ−1,q+(2ℓ+1)(2q−1)Sℓ,q−1. The displayed factorial coefficients satisfy this: the ratios are Sℓ−1,q/Sℓ+1,q=(ℓ−q)(ℓ−q+1)/[(ℓ+q)(ℓ+q+1)] and Sℓ+1,q/Sℓ,q−1=(2q−1)(ℓ+q)(ℓ+q+1)/(2q), whose difference gives the recurrence. At the top index q=ℓ+1, Sℓ+1,ℓ+1=(2ℓ+1)2Sℓ,ℓ; thus induction proves the stated sum at every degree.

3.1step 2.1F2algebra

Every Sℓm is positive, so differentiating the finite sum gives Fℓ′(z)<0. For 0≤m≤ℓ−1, Sℓm/Sℓ−1,m=(ℓ+m)/(ℓ−m)≥1, and the degree-ℓ sum has one additional positive term. Hence ∣hℓ∣ decreases with z and ∣hℓ−1∣≤∣hℓ∣. For ℓ≥1, [F2] now implies ∣hℓ′∣≤∣hℓ−1∣+(ℓ+1)∣hℓ∣/z≤(1+(ℓ+1)/z)∣hℓ∣; for ℓ=0 the same bound follows by differentiating h0=−ieiz/z.

4.1step 1.1step 2.1algebra∎

Differentiating the finite sum in step 1.1 cancels its ieiz derivative in hℓ′−ihℓ, so ∣z(hℓ′−ihℓ)∣≤∑m=0ℓ(m+1)Aℓmz−m−1. The lowest-power term of the positive modulus sum gives ∣hℓ(z0)∣≥Aℓℓz0−ℓ−1. For j=ℓ−m, factorial cancellation gives Aℓ,ℓ−jAℓℓ=2jj!∏s=0j−1ℓ−s2ℓ−s≤2jj!. Using z≥z0 and m+1≤ℓ+1, the quotient in the claim is at most (ℓ+1)∑j=0ℓ(2z0)j/j!≤(ℓ+1)e2z0.

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Exact plane-wave reflection coefficient of the local impedance condition

Statement

For 0<q≤k and tangential wavevector η∈R2 satisfying q2+∣η∣2=k2, consider u(x,y)=eiη⋅y(eiq(x−R)+Re−iq(x−R)). The impedance condition First-order local impedance condition at an artificial plane gives R=q−kq+k,∣R∣=k−qk+q. Thus reflection is zero at normal incidence q=k and its magnitude tends to one as q↓0 (grazing incidence).

Facts & Assumptions

Given: A homogeneous propagating mode with 0<q≤k and the boundary convention in [F1].

[F1]

First-order local impedance condition at an artificial plane: on x=R impose ∂xu−iku=0 with outward normal +ex.

Proof

Given: The mode and condition in [F1].

1.1givenF1algebra

At x=R, the bracket in the definition of u is 1+R and its x derivative is iq(1−R). Substitution into [F1], after cancelling the nonzero tangential exponential, gives q(1−R)−k(1+R)=0.

2.1step 1.1algebra∎

Since q+k>0, solving the equation in step 1.1 gives R=(q−k)/(q+k). The numerator is nonpositive for q≤k, so ∣R∣=(k−q)/(k+q); this is zero at q=k and tends to 1 as q↓0.

TheoremStatement: Literature-sourcedProof: AI-adaptedprecheck passjudge pass (gpt-6-luna)Open item page →

Exact reflected-mode error from a finite Dirichlet-terminated PML

Statement

For q>0, A≠0, and a finite layer 0≤x≤L with S(L)>0, let a one-dimensional mode be u(x)=AeiqX(x)+Be−iqX(x), with the PML stretch from Cartesian complex-stretch PML for a homogeneous Helmholtz mode. Imposing u(L)=0 gives the reflected amplitude at the interface BA=−e2iqX(L),∣BA∣=e−2qS(L). This is the exact continuous one-mode error for a Dirichlet termination.

Facts & Assumptions

Given: A propagating mode q>0 and finite stretch data [F1].

[F1]

Cartesian complex-stretch PML for a homogeneous Helmholtz mode: X(L)=L+iS(L); the positive and negative normal modes in the stretched coordinate are eiqX and e−iqX.

[F2]

Perfect matching and attenuation for non-grazing propagating modes: the outgoing mode is matched at the interface and attenuated by e−qS in one pass.

Proof

Given: q>0, S(L)>0, and [F1]–[F2].

1.1givenF1algebra

The condition u(L)=0 reads AeiqX(L)+Be−iqX(L)=0. Since exponentials never vanish, if A≠0 division gives B/A=−e2iqX(L).

2.1F1F2step 1.1algebra∎

With X(L)=L+iS(L), ∣e2iqX(L)∣=∣e2iqL−2qS(L)∣=e−2qS(L). The result measures the reflected-to-incident coefficient at x=0, where X(0)=0; it is the two-way attenuation through the continuous layer.

DefinitionDefinition: Literature-sourcedProof: Not applicablejudge pass (gpt-6-luna)Open item page →

Exact modal Dirichlet-to-Neumann map on a sphere

Definition

For k>0, R>0, and g∈C∞(S2;C), let gℓ be its L2(S2)-orthogonal projection onto Hℓ and set τℓ(k,R)=k(hℓ(1))′(kR)hℓ(1)(kR),Tk,Rg=∑ℓ=0∞τℓ(k,R)gℓ. The associated outgoing extension for r≥R is v(r,ω)=∑ℓ=0∞hℓ(1)(kr)hℓ(1)(kR)gℓ(ω). The denominator is nonzero by Outgoing spherical Hankel modes have positive flux and no positive-real zeros. The convergence, smoothness, PDE, and radiation properties are asserted in The spherical modal DtN map is well-defined and exact for smooth data ↗.

TheoremStatement: Literature-sourcedProof: AI-adaptedprecheck passjudge pass (gpt-6-luna)Open item page →

Exact spherical-mode reflection under the local impedance truncation

Statement

Fix k,R>0 and ℓ≥0. On r=R, write one radial mode as u(r)=Ahℓ(1)(kr)+Bhℓ(2)(kr), where hℓ(2)=hℓ(1)‾. If u satisfies ∂ru−iku=0 at R, then B=−(hℓ(1))′(kR)−ihℓ(1)(kR)(hℓ(2))′(kR)−ihℓ(2)(kR)A. The denominator is nonzero. For A≠0, the exact reflected modal-amplitude ratio is therefore BA=−(hℓ(1))′(kR)−ihℓ(1)(kR)(hℓ(2))′(kR)−ihℓ(2)(kR). If A=0, the coefficient equality forces B=0 and no ratio is defined. No uniform-in-ℓ smallness is asserted.

Facts & Assumptions

Given: The outgoing/incoming radial pair at positive real argument.

[F1]

First-order local impedance condition at an artificial plane: the spherical truncation condition uses the outgoing convention ∂ru−iku=0.

[F2]

Outgoing spherical Hankel modes have positive flux and no positive-real zeros: Im⁡(hℓ(1)‾(hℓ(1))′)=z−2 and the incoming conjugate has the negative of this flux.

Proof

Given: k,R>0, ℓ≥0, and [F1]–[F2].

1.1F1F2algebra

Let z=kR. The boundary condition, divided by k, is A((hℓ(1))′(z)−ihℓ(1)(z))+B((hℓ(2))′(z)−ihℓ(2)(z))=0. If the incoming factor in parentheses were zero, then (hℓ(2))′=ihℓ(2), so Im⁡(hℓ(2)‾(hℓ(2))′)=∣hℓ(2)∣2>0 by nonvanishing, contradicting its negative flux from [F2]. Hence that factor is nonzero.

2.1step 1.1algebra∎

Divide the equation in step 1.1 by its nonzero incoming factor to obtain the displayed coefficient equality for every A,B. For A≠0, division by A gives the displayed ratio. If A=0, the coefficient equality forces B=0, so the boundary condition has no nonzero purely incoming mode and the zero mode carries no ratio.

TheoremStatement: Literature-sourcedProof: AI-adaptedprecheck passjudge pass (gpt-6-luna)Open item page →

Rellich uniqueness for the sound-soft spherical obstacle

Statement

For a>0, k>0, and the convention in Sound-soft exterior Helmholtz problem for a spherical obstacle, every classical outgoing solution of (Δ+k2)u=0 on r>a with zero Dirichlet trace at r=a is identically zero.

Facts & Assumptions

Given: A classical outgoing u with u(a,ω)=0.

[F1]

Sound-soft exterior Helmholtz problem for a spherical obstacle: u solves the homogeneous Helmholtz equation, has zero inner trace, and satisfies r(∂r−ik)u→0 uniformly.

[F2]

Spherical harmonic modes are orthogonal, complete for continuous data, and have polynomial evaluation bounds: the degree spaces are orthogonal, their algebraic sum is uniformly dense in continuous sphere data, ordered projections of continuous data converge in L2, and the angular Laplacian is self-adjoint on smooth functions.

[F3]

Outgoing spherical Hankel modes have positive flux and no positive-real zeros: every outgoing radial mode has flux r2Im⁡(hˉℓ(kr)∂rhℓ(kr))=1/k.

[F4]

Every outgoing spherical Helmholtz mode is an outgoing Hankel mode: the degree-ℓ projection of u is cℓhℓ(1)(kr) with cℓ independent of r.

Proof

Given: The solution and supplier facts [F1]–[F4].

1.1F1F3F4algebra

By [F4], for every degree ℓ the projection of u has the form uℓ(r,⋅)=cℓhℓ(1)(kr) with cℓ independent of r. Taking the degree-ℓ projection of the zero trace at r=a gives 0=cℓhℓ(1)(ka). The nonvanishing in [F3] implies cℓ=0 for every ℓ.

2.1F2step 1.1choosealgebra∎

Thus every harmonic projection of u(r,⋅) vanishes for each r>a. By the uniform density in [F2], choose for each ε>0 a finite sum p of harmonic modes with ∥u(r,⋅)−p∥∞<ε. Orthogonality gives ⟨u,p⟩=0, so ∥u(r,⋅)∥22=∣⟨u,u−p⟩∣≤∥u(r,⋅)∥2∥u(r,⋅)−p∥2≤4πε∥u(r,⋅)∥2. Letting ε↓0 gives u(r,⋅)=0 in L2, and continuity makes it zero pointwise. Since r>a was arbitrary, u≡0.

TheoremStatement: Literature-sourcedProof: AI-adaptedprecheck passjudge pass (gpt-6-luna)Open item page →

The spherical modal DtN map is well-defined and exact for smooth data

Statement

For every k,R>0 and smooth g on S2, the series in Exact modal Dirichlet-to-Neumann map on a sphere converges in C∞(S2) to Tk,Rg, and ∣τℓ(k,R)∣≤k+(ℓ+1)/R. Its outgoing extension converges in C2 on each compact annulus R≤r≤R1, solves (Δ+k2)v=0, has trace v(R,⋅)=g and radial derivative ∂rv(R,⋅)=Tk,Rg, and satisfies the uniform outgoing Sommerfeld condition as r→∞. It is the unique classical outgoing extension of g.

Facts & Assumptions

Given: k,R>0, smooth g, and the modal definition [F1].

[F1]

Exact modal Dirichlet-to-Neumann map on a sphere: Tk,Rg=∑ℓτℓgℓ and v=∑ℓhℓ(kr)gℓ/hℓ(kR).

[F2]

Spherical harmonic modes are orthogonal, complete for continuous data, and have polynomial evaluation bounds: ∥gℓ∥2 decays faster than every inverse power of 1+ℓ, and ∥wℓ∥∞≤(2ℓ+1)/(4π)∥wℓ∥2.

[F3]

Outgoing spherical Hankel modes have positive flux and no positive-real zeros and Spherical Hankel modulus and uniform radial bounds: hℓ(kR)≠0, ∣hℓ(kr)/hℓ(kR)∣≤1 for r≥R, ∣hℓ′∣≤(1+(ℓ+1)/z)∣hℓ∣, and ∣z(hℓ′−ihℓ)∣/∣hℓ(kR)∣≤(ℓ+1)e2kR for z≥kR.

[F4]

Every outgoing spherical Helmholtz mode is an outgoing Hankel mode: every classical outgoing solution has precisely the outgoing radial mode in each degree.

[F5]

Spherical harmonic modes are orthogonal, complete for continuous data, and have polynomial evaluation bounds: Δ=∂rr+2r−1∂r+r−2ΔS2, ΔS2wℓ=−ℓ(ℓ+1)wℓ, and ∥wℓ∥Cp≤Cp(1+ℓ)p+1/2∥wℓ∥2 for every fixed p.

Proof

Given: k,R>0, g∈C∞(S2), and [F1]–[F5].

1.1F2F3F5algebra

By [F3], ∣τℓ∣≤k+(ℓ+1)/R. The Cp estimate in [F5] and the super-polynomial decay in [F2] show that for every p, ∑ℓ∥τℓgℓ∥Cp<∞. Thus the defining series converges in every smooth norm to a smooth function Tk,Rg.

2.1F1F2F3F5step 1.1algebra

For r≥R, the positive coefficient formula for ∣hℓ(z)∣2 in [F3] makes ∣hℓ(kr)/hℓ(kR)∣≤1. The derivative estimate in [F3] bounds one radial derivative of the ratio by k+(ℓ+1)/r times this ratio; repeated radial derivatives are bounded by polynomials in 1+ℓ on each compact annulus by differentiating the radial ODE in [F5]. Angular derivatives likewise contribute only polynomial factors. Thus [F2] and the evaluation bound make the extension series and its derivatives through order two uniformly convergent on R≤r≤R1. Termwise differentiation is valid; each summand solves the Helmholtz equation by [F5], its trace is gℓ, and its radial derivative at R is τℓgℓ. Summing proves the trace, derivative, and PDE claims.

3.1F1F2F3step 2.1algebra

For each fixed ℓ, the finite formula in [F3] gives r(∂r−ik)(hℓ(kr)/hℓ(kR))→0. The last bound in [F3], multiplied by ∥gℓ∥∞, dominates the absolute value of this degree's radiation residual by (ℓ+1)e2kR(2ℓ+1)/(4π)∥gℓ∥2, a summable sequence by [F2]. Dominated convergence for this series proves uniform convergence of the full radiation residual to zero.

4.1F1F2F3F4step 2.1∎

Let w be any other classical outgoing extension of g. By [F4], its degree-ℓ projection is dℓhℓ(1)(kr) for a fixed dℓ∈Hℓ. Its trace at R is gℓ, so dℓhℓ(1)(kR)=gℓ. Nonvanishing in [F3] forces dℓ=gℓ/hℓ(1)(kR), the same coefficient as the constructed extension in [F1]. Their difference has every harmonic projection zero and is continuous; density in [F2] implies the difference vanishes. This proves uniqueness and the well-definedness claimed in [F1].

DefinitionDefinition: Literature-sourcedProof: Not applicableOpen item page →

Exact-DtN truncated modal variational formulation

Definition

Fix 0<a<R and k>0. The coefficient energy space Va,R consists of sequences u=(uℓ)ℓ≥0 with uℓ∈H1((a,R);Hℓ) and ∥u∥V2=∑ℓ=0∞∫aR(r2∥uℓ′(r)∥22+(1+ℓ(ℓ+1))∥uℓ(r)∥22)dr<∞. For smooth inner data f on S2, let fℓ be its projection onto Hℓ and define the affine trial space Vf={u∈Va,R:uℓ(a)=fℓ for every ℓ} and test space V0={v∈Va,R:vℓ(a)=0 for every ℓ}. Traces and continuity of the following form are established in Modal trace bound and continuity of the exact-DtN variational form ↗. With the inner product linear in its first argument, set ak,a,R(u,v)=∑ℓ=0∞∫aR(r2⟨uℓ′,vℓ′⟩+(ℓ(ℓ+1)−k2r2)⟨uℓ,vℓ⟩)dr−R2∑ℓ=0∞τℓ(k,R)⟨uℓ(R),vℓ(R)⟩. The exact-DtN variational problem is to find u∈Vf such that ak,a,R(u,v)=0 for every v∈V0. The assigned theorem on this page proves existence and uniqueness.

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Modal trace bound and continuity of the exact-DtN variational form

Statement

Fix 0<a<R, k>0, and let Va,R and ak,a,R be as in Exact-DtN truncated modal variational formulation. There is C=C(a,R,k) such that for every u,v∈Va,R, ∑ℓ≥0(1+ℓ)(∥uℓ(a)∥22+∥uℓ(R)∥22)≤C∥u∥V2,∣ak,a,R(u,v)∣≤C∥u∥V∥v∥V. In particular, the defining traces and boundary pairing are finite, the form is continuous, Va,R is a Hilbert direct sum, and finite-degree truncations converge in its norm.

Facts & Assumptions

Given: The annulus 0<a<R, fixed k>0, and the energy space and form [F1].

[F1]

Exact-DtN truncated modal variational formulation: uℓ∈H1((a,R);Hℓ) with squared energy weighted by r2 and 1+ℓ(ℓ+1); the boundary coefficient satisfies τℓ=khℓ′(kR)/hℓ(kR).

[F2]

The spherical modal DtN map is well-defined and exact for smooth data: for fixed k,R, ∣τℓ∣≤k+(ℓ+1)/R.

Proof

Given: u,v∈Va,R and [F1]–[F2].

1.1F1algebra

Each H1((a,R);Hℓ) is complete because Hℓ is finite dimensional. A Cauchy sequence in the weighted square-sum norm is Cauchy in each coordinate; take its coordinatewise H1 limits. For every finite number of coordinates the squared norm of the limit is bounded by the liminf of the sequence norms, so the coordinatewise limit has finite total norm; applying the same argument to differences shows convergence in the sum norm. Tails of the defining convergent nonnegative series tend to zero, so finite-degree truncations are dense. For any scalar or finite-dimensional Hilbert-valued w∈H1(a,R), set A=∥w∥L2(a,R) and B=∥w′∥L2(a,R). Absolute continuity and ∣w(R)∣2−∣w(t)∣2=2Re⁡∫tR⟨w′(s),w(s)⟩ds give, after averaging t over [a,R] and applying Cauchy–Schwarz, ∥w(R)∥2≤(R−a)−1A2+2AB. Multiplying by 1+ℓ and using 2(1+ℓ)AB≤(1+ℓ)2A2+B2, (1+ℓ)2≤2(1+ℓ(ℓ+1)), and B2≤a−2∫aRr2∥w′∥2dr gives (1+ℓ)∥w(R)∥2≤Ca,R∫aR(r2∥w′∥2+(1+ℓ(ℓ+1))∥w∥2)dr. Replacing r by a+R−r proves the same inequality at the inner endpoint. Summing with w=uℓ proves the weighted trace estimate.

2.1F1F2step 1.1algebra∎

The volume terms of a are bounded by a constant times ∥u∥V∥v∥V because r lies in [a,R] and k is fixed. By [F2], ∣τℓ∣≤Ck,R(1+ℓ). Cauchy–Schwarz over degrees and the trace estimate from step 1.1 give ∑ℓ∣τℓ⟨uℓ(R),vℓ(R)⟩∣≤C(∑ℓ(1+ℓ)∥uℓ(R)∥22)1/2(∑ℓ(1+ℓ)∥vℓ(R)∥22)1/2≤C∥u∥V∥v∥V. Thus the boundary series is absolutely convergent and the whole form is continuous.

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Existence and uniqueness for the spherical exact-DtN variational problem

Statement

Fix 0<a<R, k>0, and smooth f on S2. The exact-DtN variational problem of Exact-DtN truncated modal variational formulation has exactly one solution u∈Vf. It is the restriction to a≤r≤R of the outgoing modal field u(r,ω)=∑ℓ=0∞hℓ(1)(kr)hℓ(1)(ka)fℓ(ω), where fℓ is the degree-ℓ projection of f.

Facts & Assumptions

Given: 0<a<R, k>0, smooth f, and the variational definition [F1].

[F1]

Exact-DtN truncated modal variational formulation: the trial trace at a is fℓ, tests have zero trace at a, and the form subtracts R2τℓ at the outer boundary.

[F2]

Modal trace bound and continuity of the exact-DtN variational form: the form and traces are continuous on the coefficient energy space; finite-degree tests are dense by truncating the defining Hilbert sum.

[F3]

The spherical modal DtN map is well-defined and exact for smooth data: the outgoing modal series for smooth data at any positive sphere is classical, solves the Helmholtz equation, has the prescribed trace, and satisfies uℓ′(R)=τℓuℓ(R).

[F4]

Spherical harmonic modes are orthogonal, complete for continuous data, and have polynomial evaluation bounds: ∥fℓ∥2 decays faster than every inverse power of 1+ℓ and the degree-ℓ angular energy is ℓ(ℓ+1) times the squared L2 norm.

[F5]

Outgoing spherical Hankel modes have positive flux and no positive-real zeros and Spherical Hankel modulus and uniform radial bounds: hℓ(1)(ka)≠0, the outgoing/incoming Wronskian is nonzero, ∣hℓ(kr)/hℓ(ka)∣≤1 for r≥a, and ∣hℓ′∣≤(1+(ℓ+1)/(kr))∣hℓ∣.

Proof

Given: The data and suppliers [F1]–[F4].

1.1F1F3F4F5algebra

By [F3] applied at the inner radius a, the proposed series has inner trace f. Its degree-ℓ radial ratio has modulus at most one for r≥a by [F5], and its radial derivative is bounded by k+(ℓ+1)/r times that ratio. The angular energy of degree ℓ is ℓ(ℓ+1) times its squared L2 norm. Consequently its total V energy is at most Ca,R,k∑ℓ(1+ℓ)2∥fℓ∥22, which is finite by [F4]. Thus it belongs to Vf.

1.2F1F2algebra

Let w∈V0 solve the homogeneous variational equation. Testing against functions supported in a single degree and compactly supported in (a,R) shows distributionally that (r2wℓ′)′+(k2r2−ℓ(ℓ+1))wℓ=0. Since the coefficients are smooth and r>0, this one-dimensional equation implies wℓ∈C2([a,R];Hℓ). Integrating by parts and allowing arbitrary outer test trace yields wℓ′(R)=τℓwℓ(R); the inner trace is wℓ(a)=0.

2.1F1F2F3step 1.1algebra

Each modal coefficient satisfies (r2uℓ′)′+(k2r2−ℓ(ℓ+1))uℓ=0 and uℓ′(R)=τℓuℓ(R) by [F3]. Integration by parts against a finite-degree test with zero inner trace makes its modal volume term equal R2uℓ′(R)vℓ(R)‾; the outer term in [F1] subtracts exactly R2τℓuℓ(R)vℓ(R)‾. Hence the form vanishes for every finite-degree test. Finite-degree truncations converge in V, and [F2] extends the identity to every test in V0. This proves existence.

3.1F1F5step 1.2algebra∎

The radial ODE solution is wℓ(r)=Aℓhℓ(1)(kr)+Bℓhℓ(2)(kr): the two solutions have nonzero Wronskian by [F5], and matching value and derivative at one radius followed by uniqueness of the linear initial-value equation spans all solutions. At R, the condition from step 1.2 gives Bℓk((hℓ(2))′(kR)−[(hℓ(1))′(kR)/hℓ(1)(kR)]hℓ(2)(kR))=0. The parenthesized factor is the nonzero Wronskian divided by hℓ(1)(kR), so Bℓ=0. The inner condition and [F5] then give Aℓ=0. Every modal projection vanishes, hence w=0 in V. This proves uniqueness.

5 · Examples, counterexamples and false statements

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