Endpoint spaces and flat energy shells

Written by GPT-6.1 Sol (OpenAI) and GPT-6 Astra (OpenAI). Self-checked by the writing AI. Original exposition: CC0. The linked coordinate supplement retains CC BY-SA 4.0.

Working question: Which norm can retain a radiating tail? A wave whose squared mass on a ball grows like its radius can have a nonzero far-field amplitude while failing to belong to L2L^2. The explicit transport solution in the course guide lets you see the tail before introducing the dyadic norm. The issue is whether an observation discards that tail, not whether the wave becomes pointwise small.

An outgoing wave can have an amount of squared mass proportional to the radius of a ball. Ordinary L2L^2 excludes such a wave. A dyadic spatial norm permits this growth while still pairing the wave with a sufficiently localized forcing term. The same norm makes sense of restricting a Fourier transform to an energy shell.

The Fourier and measure inputs have the exact prerequisite proofs specified in Section 1. Hilbert representation and the shell dualities are proved below; the full Hahn–Banach input for infinite codimension has its separate programme locator. Resolvents, domains and spectral density explains why a real-energy solution needs a specified topology. The freely readable Agmon lectures [A], Section 1, equations (1.5)–(1.9), define the same shell and vanishing-mass spaces, with an equivalent ball norm on the dual. The exact dyadic norm constants, infinite-codimension bidual argument, logarithmic criterion and transport statements used here are proved below; the lecture notes are not a proof of those refinements. Yafaev [Y] and Teschl [T] give freely accessible scattering background. We first solve the flat-shell model completely, including the difference between weak-star and norm convergence. The exact tail-shell distance measures the obstruction: a nonzero Fourier trace leaves persistent mass at infinity. Each trace is strongly continuous in energy on a fixed forcing term, although the trace operators are nowhere continuous in operator norm. Fourier traces on curved energy surfaces then treats graph patches and their surface-layer mass.

The earlier flat transport reading supplies the complete shell, trace and transport proofs used by the first spectral lesson. Those arguments are retained here alongside the bidual and weighted refinements. For the integral and elementary-calculus steps, read Banach-valued integration, real powers and logarithms, the continuous scalar fundamental theorem, and polar integration. Weighted Hilbert duality is proved in the first spectral lesson, Section 5.

1. Measuring one shell at a time

Read the Euclidean product and Fourier proofs, in the order specified there, before this lesson. They prove the integration, smooth density, Gaussian transform and Plancherel facts used below. Multiplying that reading's forward Fourier transform by (2π)−n/2(2\pi)^{-n/2} gives our unitary convention.

Hilbert representation and separation used below. If CC is a nonempty closed convex subset of a Hilbert space and d=inf⁡c∈C∥x−c∥d=\inf_{c\in C}\|x-c\|, a minimizing sequence cjc_j satisfies ∥cj−ck∥2=2∥x−cj∥2+2∥x−ck∥2−4∥x−cj+ck2∥2⟶0. \|c_j-c_k\|^2 =2\|x-c_j\|^2+2\|x-c_k\|^2 -4\left\|x-\frac{c_j+c_k}{2}\right\|^2\longrightarrow0. The midpoint belongs to CC, so its squared distance is at least d2d^2. Completeness and closedness give a minimizing point cc. For every z∈Cz\in C, compare cc with c+t(z−c)c+t(z-c), 0<t≤10<t\le1, expand the squared distance, divide by tt and let t↓0t\downarrow0. The result is Re⁡(x−c,z−c)≤0\operatorname{Re}(x-c,z-c)\le0. If x∉Cx\notin C, this separates xx strictly from CC. If CC is a closed linear subspace, use z=c+tvz=c+tv and z=c+itvz=c+itv, with both signs of real tt, to obtain x−c⊥Cx-c\perp C.

For a nonzero bounded linear functional ℓ\ell, apply this projection to its closed kernel and to a vector outside that kernel. Normalize its nonzero orthogonal residual to a unit vector ee. For each xx, the vector x−ℓ(x)e/ℓ(e)x-\ell(x)e/\ell(e) lies in the kernel; orthogonality gives ℓ(x)=ℓ(e)(x,e)\ell(x)=\ell(e)(x,e). Thus ℓ(x)=(x,ℓ(e)‾e)\ell(x)=(x,\overline{\ell(e)}e), with representing-vector norm exactly ∥ℓ∥\|\ell\|. The zero functional has the zero representative, and testing their difference proves uniqueness. This supplies the Hilbert representation used on every shell. The same projection proof supplies the separation of closed convex subsets of a Hilbert space used in the onto criterion.

Set Rj=2jR_j=2^j,

A0={∣x∣<1},Aj={2j−1≤∣x∣<2j}(j≥1). A_0=\{|x|<1\},\qquad A_j=\{2^{j-1}\leq|x|<2^j\}\quad(j\geq1).

Boundary spheres have measure zero and play no role. Indeed a sphere of radius r>0r>0 is contained in every shell r−δ<∣x∣<r+δr-\delta<|x|<r+\delta. The change-of-variables formula gives ∣BR∣=Rn∣B1∣|B_R|=R^n|B_1|, so the volumes of these shells tend to zero with δ\delta. The unit ball has finite volume because it lies in a bounded cube. Define

∥f∥B=∑j≥0Rj1/2∥f∥L2(Aj),∥u∥B∗=sup⁡j≥0Rj−1/2∥u∥L2(Aj). \|f\|_B=\sum_{j\geq0}R_j^{1/2}\|f\|_{L^2(A_j)}, \qquad \|u\|_{B^*}=\sup_{j\geq0}R_j^{-1/2}\|u\|_{L^2(A_j)}.

The spaces BB and B∗B^* contain exactly the locally square-integrable functions with finite indicated norms. The star denotes the integral dual, not a Sobolev exponent.

Theorem 1.1. Both spaces are Banach. The pairing

(f,u)=∫f(x)u(x)‾ dx (f,u)=\int f(x)\overline{u(x)}\,dx

identifies every continuous linear functional on BB with a unique u∈B∗u\in B^*, and its norm is exactly ∥u∥B∗\|u\|_{B^*}. Smooth compactly supported functions are dense in BB.

Proof. Map ff to the sequence (Rj1/2f∣Aj)j(R_j^{1/2}f|_{A_j})_j. This is an isometric bijection from BB to the ℓ1\ell^1 sum of the Hilbert spaces L2(Aj)L^2(A_j); the corresponding ℓ∞\ell^\infty sum represents B∗B^*. For completeness, each component of a Cauchy sequence converges in its Hilbert space. Once two sequence indices are large, the norm of their difference is at most ε\varepsilon. Pass to the component limit on each finite set of indices, then take the supremum over those finite sets. This bounds the sum, or the supremum, of the limiting difference by ε\varepsilon. Comparing with one fixed sequence member gives a finite norm for the limit and proves convergence in the claimed space.

Cauchy–Schwarz on every shell proves ∣(f,u)∣≤∥f∥B∥u∥B∗|(f,u)|\leq\|f\|_B\|u\|_{B^*}. Conversely, the restriction of a functional to each one-shell Hilbert space is represented by a unique vector uju_j; its norm bound says Rj−1/2∥uj∥2≤∥ℓ∥R_j^{-1/2}\|u_j\|_2\leq\|\ell\|. Join these vectors into uu. Finite shell sums have the claimed representation, and their density in the ℓ1\ell^1 sum extends it to all BB. Testing with a unit vector supported in one shell, and taking the supremum over shells, proves the exact norm equality and uniqueness.

For density, first discard all shells beyond a finite index; their BB norm tends to zero. The truncated function is supported in a fixed ball. Approximate it in L2L^2 by smooth functions supported in a slightly larger ball. Only finitely many shells then occur, so their BB norm is bounded by a fixed constant times the L2L^2 error. □\square

The same proof shows B⊂L2B\subset L^2, since ∥f∥2≤∑j∥f∥L2(Aj)≤∥f∥B\|f\|_2\leq\sum_j\|f\|_{L^2(A_j)}\leq\|f\|_B.

2. The waves that carry no mass at infinity

Define B0∗B^*_0 by the additional condition

Rj−1/2∥u∥L2(Aj)⟶0. R_j^{-1/2}\|u\|_{L^2(A_j)}\longrightarrow0.

Theorem 2.1. For u∈B∗u\in B^*,

∥u∥B∗2≤sup⁡R≥11R∫∣x∣<R∣u∣2 dx≤4∥u∥B∗2. \|u\|_{B^*}^2\leq \sup_{R\geq1}\frac1R\int_{|x|<R}|u|^2\,dx \leq4\|u\|_{B^*}^2.

Moreover u∈B0∗u\in B^*_0 exactly when

1R∫∣x∣<R∣u∣2 dx⟶0. \frac1R\int_{|x|<R}|u|^2\,dx\longrightarrow0.

The space B0∗B^*_0 is the B∗B^*-norm closure of Cc∞C_c^\infty, and its continuous dual is BB under the integral pairing.

Proof. For each jj, the shell integral divided by RjR_j is at most the ball integral with radius RjR_j divided by RjR_j. This proves the first inequality. Choose jj with Rj−1<R≤RjR_{j-1}<R\leq R_j, or j=0j=0 when R=1R=1. The ball is contained in the union of shells with index at most jj, and

∫∣x∣<R∣u∣2≤∥u∥B∗2∑k=0jRk≤2Rj∥u∥B∗2≤4R∥u∥B∗2. \int_{|x|<R}|u|^2\leq \|u\|_{B^*}^2\sum_{k=0}^jR_k \leq2R_j\|u\|_{B^*}^2\leq4R\|u\|_{B^*}^2.

If the ball quotient tends to zero, the shell quotients do too. Conversely, split the ball integral into finitely many early shells and the tail. The early integral divided by RR tends to zero, while if each tail shell quotient is at most δ2\delta^2, the preceding geometric sum bounds the tail ball quotient by 4δ24\delta^2. Let δ↓0\delta\downarrow0.

Truncation to finitely many shells converges in B∗B^* exactly under this vanishing condition. Approximation in L2L^2 on a fixed ball then gives smooth compactly supported approximants as in Theorem 1.1. Conversely, every such smooth function has vanishing tails, and the vanishing-tail subspace is norm closed.

Finally B0∗B^*_0 is the c0c_0 sum of the weighted shell Hilbert spaces. To see its dual explicitly, restrict a functional to the individual components. If those restrictions have norms aja_j, choose finitely many unit component vectors whose functional values are nonnegative real and arbitrarily close to aja_j. Their combined vector has supremum norm one, giving ∑j≤Naj≤∥ℓ∥\sum_{j\leq N}a_j\leq\|\ell\|. Hence (aj)∈ℓ1(a_j)\in\ell^1. The Hilbert representatives therefore combine into a vector of BB. Finite component sums are dense in c0c_0, so the representation extends to every vector. The reverse bound and exact norm follow by the same test. □\square

Every L2L^2 function belongs to B0∗B^*_0. A function with a nonzero average mass per unit radius does not. The distinction between B∗B^* and B0∗B^*_0 is essential in radiation conditions.

Example 2.2. In dimension nn, let u(x)=∣x∣−(n−1)/2u(x)=|x|^{-(n-1)/2} for ∣x∣≥1|x|\geq1, and set it to zero inside the unit ball. Then ∫Aj∣u∣2 dx=∣Sn−1∣2j−1\int_{A_j}|u|^2\,dx=|\mathbb S^{n-1}|2^{j-1}. Thus u∈B∗u\in B^*, while the ball quotient tends to ∣Sn−1∣|\mathbb S^{n-1}|, so u∉B0∗u\notin B^*_0. Multiplication by a complex factor of modulus one does not change these conclusions.

The inclusions Cc∞⊂S⊂L2⊂B0∗C_c^\infty\subset\mathcal S\subset L^2\subset B^*_0, together with Theorem 2.1, show that the closures of both S\mathcal S and L2L^2 in B∗B^* are exactly B0∗B^*_0. The dual of this vanishing-tail space recovers BB. The full bidual is much larger.

Proposition 2.3. The canonical image of BB is a closed subspace of infinite codimension in its bidual. In particular BB is not reflexive.

Proof. Keep the complex-linear dual convention explicit. Write B′B' for the space of bounded complex-linear functionals on BB. Theorem 1.1 identifies each of them with

ℓu(f)=(f,u),u∈B∗. \ell_u(f)=(f,u),\qquad u\in B^*.

This parametrization is conjugate-linear in uu, since our integral pairing is linear in its first argument. We work with the actual linear dual B′B' and its dual B′′B''. The canonical map is

J:B⟶B′′,(Jf)(ℓ)=ℓ(f). J:B\longrightarrow B'',\qquad (Jf)(\ell)=\ell(f).

Theorem 1.1 gives ∥Jf∥=∥f∥B\|Jf\|=\|f\|_B: its upper bound is the dual norm estimate; for the reverse bound, choose on each nonzero shell the representing vector in the direction of ff, with L2L^2 norm Rj1/2R_j^{1/2}. The resulting uu has B∗B^* norm at most one and (f,u)=∑jRj1/2∥f∥L2(Aj)(f,u)=\sum_jR_j^{1/2}\|f\|_{L^2(A_j)}. Completeness of BB then makes J(B)J(B) closed. Indeed a convergent sequence JfkJf_k makes fkf_k Cauchy by the isometry, and its limit maps to the original limit.

Choose a unit vector ej∈L2(Aj)e_j\in L^2(A_j) for each shell and put vj=Rj−1/2ej∈Bv_j=R_j^{-1/2}e_j\in B, extended by zero off that shell. The map

Q:B′⟶ℓ∞,Qℓ=(ℓ(vj))j≥0 Q:B'\longrightarrow\ell^\infty,\qquad Q\ell=(\ell(v_j))_{j\geq0}

is linear and has norm at most one because ∥vj∥B=1\|v_j\|_B=1. It is onto: for a=(aj)∈ℓ∞a=(a_j)\in\ell^\infty, the function whose shell restriction is Rj1/2aj‾ejR_j^{1/2}\overline{a_j}e_j has B∗B^* norm ∥a∥∞\|a\|_\infty, and its functional has Qℓu=aQ\ell_u=a. Define

D0={ℓu:u∈B0∗}⊂B′. D_0=\{\ell_u:u\in B^*_0\}\subset B'.

Then Q(D0)⊂c0Q(D_0)\subset c_0. Here c0c_0 denotes the scalar sequences tending to zero, with the supremum norm.

For r≥1r\geq1, take the pairwise disjoint infinite index sets

Ir={2r−1(2m−1):m≥1},br=1Ir∈ℓ∞. I_r=\{2^{r-1}(2m-1):m\geq1\},\qquad b_r=\mathbf1_{I_r}\in\ell^\infty.

On the linear subspace

E=c0+span⁡{br:r≥1} E=c_0+\operatorname{span}\{b_r:r\geq1\}

define hr(c+∑sαsbs)=αrh_r(c+\sum_s\alpha_s b_s)=\alpha_r, where every sum is finite. Along indices in IsI_s tending to infinity, the sequence in parentheses tends to αs\alpha_s. Thus the coefficients are unique, and

∥c+∑sαsbs∥∞≥max⁡s∣αs∣. \left\|c+\sum_s\alpha_s b_s\right\|_\infty \geq\max_s|\alpha_s|.

Each hrh_r is consequently a complex-linear functional of norm one. The full Hahn–Banach theorem, proved in Hahn–Banach, Baire and the basic theorems on Banach spaces, Theorems 2.1–2.2 and Corollary 2.3, extends it to a norm-one functional HrH_r on ℓ∞\ell^\infty. That theorem permits an arbitrary subspace; EE is not a finite-dimensional domain. Section 1 proves Zorn's lemma from the axiom of choice, and Section 2 proves the real extension and complex reduction.

Set Φr=Hr∘Q∈B′′\Phi_r=H_r\circ Q\in B''. It annihilates D0D_0. Let usu_s have restriction Rj1/2ejR_j^{1/2}e_j on shells indexed by IsI_s, and zero on all other shells. Then

∥us∥B∗=1,Qℓus=bs,Φr(ℓus)=δrs. \|u_s\|_{B^*}=1,\qquad Q\ell_{u_s}=b_s,\qquad \Phi_r(\ell_{u_s})=\delta_{rs}.

In particular these bidual functionals are linearly independent and each has norm one. More is needed for codimension: no nonzero JfJf can annihilate D0D_0. Tests uu supported in one shell belong to B0∗B^*_0; if all (f,u)(f,u) vanish, each shell restriction of ff is zero. Hence

J(B)∩{Φ∈B′′:Φ∣D0=0}={0}. J(B)\cap\{\Phi\in B'':\Phi|_{D_0}=0\}=\{0\}.

If a finite sum ∑rβrΦr\sum_r\beta_r\Phi_r belongs to J(B)J(B), this intersection makes the sum zero, and testing on ℓus\ell_{u_s} gives βs=0\beta_s=0 for every index in the sum. The cosets of the Φr\Phi_r in B′′/J(B)B''/J(B) are therefore linearly independent. The quotient has infinite dimension, proving both assertions. □\square

The functionals Φr\Phi_r vanish on every vanishing-tail wave, while detecting the persistent mass on separate infinite families of shells. This explains why testing only with B0∗B^*_0 recovers the localized forcing space BB, but does not describe every functional on the full dual.

Proposition 2.4 (exact distance to vanishing tails). For every u∈B∗u\in B^*,

dist⁡B∗(u,B0∗)=lim sup⁡j→∞Rj−1/2∥u∥L2(Aj). \operatorname{dist}_{B^*}(u,B^*_0) =\limsup_{j\to\infty}R_j^{-1/2}\|u\|_{L^2(A_j)}.

If the ball average has a limit LL, then

lim⁡R→∞1R∫∣x∣<R∣u∣2 dx=L⟹dist⁡B∗(u,B0∗)=L/2. \lim_{R\to\infty}\frac1R\int_{|x|<R}|u|^2\,dx=L \quad\Longrightarrow\quad \operatorname{dist}_{B^*}(u,B^*_0)=\sqrt{L/2}.

Proof. For v∈B0∗v\in B^*_0, the reverse triangle inequality on each shell gives

∥u−v∥B∗≥Rj−1/2∥u∥L2(Aj)−Rj−1/2∥v∥L2(Aj). \|u-v\|_{B^*}\geq R_j^{-1/2}\|u\|_{L^2(A_j)}-R_j^{-1/2}\|v\|_{L^2(A_j)}.

Take the limsup; the second term tends to zero. This proves the lower bound for every vv. For the reverse bound, truncate uu to the shells with index at most NN. This locally square-integrable, compactly supported truncation belongs to B0∗B^*_0, and its error has norm exactly sup⁡j>NRj−1/2∥u∥L2(Aj)\sup_{j>N}R_j^{-1/2}\|u\|_{L^2(A_j)}. Let N→∞N\to\infty.

Write q(R)=R−1∫∣x∣<R∣u∣2q(R)=R^{-1}\int_{|x|<R}|u|^2. For j≥1j\geq1, the squared shell norm is

Rj−1∥u∥L2(Aj)2=q(Rj)−12q(Rj/2)⟶L/2. R_j^{-1}\|u\|_{L^2(A_j)}^2 =q(R_j)-\tfrac12q(R_j/2)\longrightarrow L/2.

The factor one half comes from the inner radius of our dyadic shell. Taking square roots proves the second assertion. □\square

3. Why the exponent one half is an endpoint

Write Ls2={f:⟨x⟩sf∈L2}L^2_s=\{f:\langle x\rangle^sf\in L^2\}.

Series comparisons used in the endpoint tests. If a positive function FF is decreasing for t≥Nt\geq N, then F(j+1)≤∫jj+1F(t) dt≤F(j)(j≥N). F(j+1)\leq\int_j^{j+1}F(t)\,dt\leq F(j) \qquad(j\geq N). Summing the inequalities and passing to increasing limits proves that its series and improper integral converge together. The proved real-power derivative gives the primitive t1−a/(1−a)t^{1-a}/(1-a) for t−at^{-a}, a≠1a\ne1, and the logarithm gives the primitive at a=1a=1. Thus ∑j−a\sum j^{-a} converges exactly for a>1a>1; for a≤0a\leq0 the terms do not even tend to zero. For any real qq, the function F(t)=1/[t(log⁡t)q]F(t)=1/[t(\log t)^q], t>1t>1, is eventually decreasing, since its logarithmic derivative is −(1+q/log⁡t)/t-(1+q/\log t)/t. The substitution s=log⁡ts=\log t turns its integral into ∫s−qds\int s^{-q}ds. Hence ∑j≥21j(log⁡j)q<∞⟺q>1. \sum_{j\geq2}\frac1{j(\log j)^q}<\infty \quad\Longleftrightarrow\quad q>1. Replacing jj by 1+j1+j or log⁡j\log j by log⁡(e+j)\log(e+j) changes these comparisons only by fixed positive constants. The geometric-series formula was proved in the elementary-function reading. These facts justify all the convergent and divergent series below, including the two logarithmic borderlines.

Proposition 3.1. For every s>1/2s>1/2,

Ls2⊂B⊂L2⊂B0∗⊂B∗⊂L−s2, L^2_s\subset B\subset L^2\subset B^*_0\subset B^*\subset L^2_{-s},

continuously. Neither outer inclusion remains valid with s=1/2s=1/2.

Proof. On AjA_j, ⟨x⟩\langle x\rangle is comparable to RjR_j, uniformly in jj. Cauchy–Schwarz gives

∑jRj1/2∥f∥L2(Aj)≤Cs(∑jRj1−2s)1/2∥f∥Ls2. \sum_jR_j^{1/2}\|f\|_{L^2(A_j)} \leq C_s\left(\sum_jR_j^{1-2s}\right)^{1/2}\|f\|_{L^2_s}.

The geometric sum converges exactly for s>1/2s>1/2. Similarly,

∥u∥L−s22≤Cs∑jRj−2s∥u∥L2(Aj)2≤Cs∥u∥B∗2∑jRj1−2s. \|u\|_{L^2_{-s}}^2 \leq C_s\sum_jR_j^{-2s}\|u\|_{L^2(A_j)}^2 \leq C_s\|u\|_{B^*}^2\sum_jR_j^{1-2s}.

The middle inclusions were proved above. To disprove L1/22⊂BL^2_{1/2}\subset B, choose unit L2(Aj)L^2(A_j) vectors eje_j and set f=∑j≥1Rj−1/2j−1ejf=\sum_{j\geq1}R_j^{-1/2}j^{-1}e_j. Its weighted squared norm is comparable to ∑j−2\sum j^{-2}, but its BB norm is ∑j−1\sum j^{-1}. To disprove B∗⊂L−1/22B^*\subset L^2_{-1/2}, set u=∑j≥1Rj1/2eju=\sum_{j\geq1}R_j^{1/2}e_j. Its B∗B^* norm is one, while its weighted squared norm is comparable to ∑1\sum1. □\square

4. Slicing space and tracing Fourier space

Write x=(t,y)∈R×Rn−1x=(t,y)\in\mathbb R\times\mathbb R^{n-1}.

Lemma 4.1. Every f∈Bf\in B satisfies

∫R∥f(t,⋅)∥Ly2 dt≤2∥f∥B. \int_{\mathbb R}\|f(t,\cdot)\|_{L^2_y}\,dt\leq\sqrt2\|f\|_B.

Every u∈L∞(Rt;Ly2)u\in L^\infty(\mathbb R_t;L^2_y) satisfies

∥u∥B∗≤2ess supt∥u(t,⋅)∥2. \|u\|_{B^*}\leq\sqrt2\mathop{\mathrm{ess\,sup}}_t\|u(t,\cdot)\|_2.

Proof. Let fj=f1Ajf_j=f1_{A_j}. Its slices vanish when ∣t∣>Rj|t|>R_j. Cauchy–Schwarz in tt, followed by Fubini, gives

∫∥fj(t,⋅)∥2 dt≤(2Rj)1/2∥fj∥2. \int\|f_j(t,\cdot)\|_2\,dt\leq(2R_j)^{1/2}\|f_j\|_2.

Sum this inequality and use the triangle inequality in Ly2L^2_y. For uu, integrate its slice bound on [−Rj,Rj][-R_j,R_j] to obtain ∥u∥L2(Aj)2≤2Rjsup⁡t∥u(t,⋅)∥22\|u\|_{L^2(A_j)}^2\leq2R_j\sup_t\|u(t,\cdot)\|_2^2. □\square

The unitary Fourier convention is the one proved in the earlier Fourier reading. The partial Fourier transform in yy, denoted Fy\mathcal F_y, is unitary on the slice Hilbert space. The Hilbert-valued integrals here can be constructed from simple functions: set ∫∑j1Ejvj=∑j∣Ej∣vj\int\sum_j1_{E_j}v_j=\sum_j|E_j|v_j for disjoint measurable sets of finite measure, and use ∥∫g∥≤∫∥g∥\|\int g\|\le\int\|g\| to extend by completion in L1(R;H)L^1(\mathbb R;\mathcal H). This also proves continuity of the integral and permits scalar dominated convergence applied to the norm of an error. The slice functions used here are strongly measurable: approximation of an L2L^2 function by finite rectangle simple functions, followed by a subsequence whose squared L2L^2 errors are summable, gives almost-everywhere convergence in the slice Hilbert space by Tonelli. A bounded partial Fourier transform preserves this measurability. Lemma 4.1 gives their integrable slice norm, so the construction applies. For λ∈R\lambda\in\mathbb R, define the flat-shell trace by this integral:

Tλf(η)=(2π)−1/2∫Re−itλ(Fyf)(t,η) dt. T_\lambda f(\eta) =(2\pi)^{-1/2}\int_{\mathbb R} e^{-it\lambda}(\mathcal F_yf)(t,\eta)\,dt.

Theorem 4.2. The map Tλ:B→L2(Rn−1)T_\lambda:B\to L^2(\mathbb R^{n-1}) is bounded and onto, with norm at most π−1/2\pi^{-1/2}, uniformly in λ\lambda. For each f∈Bf\in B, λ↦Tλf\lambda\mapsto T_\lambda f is continuous in L2L^2, and it agrees with Ff(λ,η)\mathcal Ff(\lambda,\eta) for Schwartz functions. Its restriction to any measurable set KK of the η\eta variables is onto L2(K)L^2(K). For n=1n=1, the target is C\mathbb C.

Proof. Minkowski's integral inequality, slice Plancherel and Lemma 4.1 give the bound. Dominated convergence for the Bochner integral gives continuity. Fubini proves the agreement on Schwartz functions.

For surjectivity on bounded KK, put

Eλa(t,y)=(2π)−1/2eitλFy−1(1Ka)(y). E_\lambda a(t,y)=(2\pi)^{-1/2}e^{it\lambda}\mathcal F_y^{-1}(1_Ka)(y).

The pairing satisfies (Tλf,a)L2(K)=(f,Eλa)(T_\lambda f,a)_{L^2(K)}=(f,E_\lambda a), first for test functions and then by density. Lemma 4.1 shows ∥Eλa∥B∗≤π−1/2∥a∥2\|E_\lambda a\|_{B^*}\leq\pi^{-1/2}\|a\|_2. A lower bound is also needed. Write v=Fy−1(1Ka)v=\mathcal F_y^{-1}(1_Ka). For each R≥1R\geq1,

1R∫∣x∣<R∣Eλa∣2 dx=1π∫∣y∣<R1−∣y∣2/R2 ∣v(y)∣2 dy. \frac1R\int_{|x|<R}|E_\lambda a|^2\,dx =\frac1\pi\int_{|y|<R} \sqrt{1-|y|^2/R^2}\,|v(y)|^2\,dy.

Dominated convergence gives the limit π−1∥a∥22\pi^{-1}\|a\|_2^2. Proposition 2.4 gives the exact quotient distance and hence the stronger lower bound

dist⁡B∗(Eλa,B0∗)=(2π)−1/2∥a∥2≤∥Eλa∥B∗. \operatorname{dist}_{B^*}(E_\lambda a,B^*_0) =(2\pi)^{-1/2}\|a\|_2 \leq\|E_\lambda a\|_{B^*}.

This argument did not use boundedness of KK, so it holds for every measurable KK, including Rn−1\mathbb R^{n-1}. The exact equality concerns distance to the vanishing-tail subspace; no equality for the ordinary B∗B^* norm is asserted.

Here is the Banach-space implication, including the onto assertion. If a bounded map T:X→HT:X\to\mathcal H, with XX Banach and H\mathcal H Hilbert, has ∥T∗a∥≥c∥a∥\|T^*a\|\geq c\|a\|, then TT is onto. Put C=T({∥x∥≤1})‾C=\overline{T(\{\|x\|\leq1\})}. It is closed, convex and balanced, and its support function in direction aa is ∥T∗a∥\|T^*a\|: multiplying an input by a unit complex scalar turns the modulus of its pairing into its real part. If some hh with ∥h∥≤c\|h\|\le c were outside CC, the closest-point separation proved in Section 1 would give a nonzero aa with sup⁡v∈CRe⁡(v,a)<Re⁡(h,a)≤c∥a∥\sup_{v\in C}\operatorname{Re}(v,a)<\operatorname{Re}(h,a)\le c\|a\|, contradicting the lower bound. Thus CC contains that ball. For any target hh, closure and scaling give x1x_1 with ∥x1∥≤2∥h∥/c\|x_1\|\leq2\|h\|/c and ∥h−Tx1∥≤∥h∥/2\|h-Tx_1\|\leq\|h\|/2. Repeat on the residual. The resulting series ∑xj\sum x_j converges in XX, has norm at most 4∥h∥/c4\|h\|/c, and its image is hh. Apply this to TλT_\lambda and the extension just constructed. It proves surjectivity on the entire flat hyperplane, and hence all the claimed special cases. For n=1n=1, the slice space is C\mathbb C and the same argument applies. □\square

Proposition 4.3 (trace operators remain separated). If λ≠μ\lambda\ne\mu, then

∥Tλ−Tμ∥B→L2≥π−1/2. \|T_\lambda-T_\mu\|_{B\to L^2}\geq\pi^{-1/2}.

Thus the family is nowhere continuous in operator norm, even though Theorem 4.2 proves continuity on each fixed ff.

Proof. Choose aa of L2L^2 norm one, put v=Fy−1av=\mathcal F_y^{-1}a, and set

w(t,y)=(Eλ−Eμ)a=(2π)−1/2(eitλ−eitμ)v(y). w(t,y)=(E_\lambda-E_\mu)a =(2\pi)^{-1/2}(e^{it\lambda}-e^{it\mu})v(y).

Let δ=λ−μ≠0\delta=\lambda-\mu\ne0 and bR(y)=R2−∣y∣2b_R(y)=\sqrt{R^2-|y|^2} on ∣y∣<R|y|<R. Integration over −bR<t<bR-b_R<t<b_R gives exactly

1R∫∣x∣<R∣w∣2 dx=12π∫∣y∣<R(4bR(y)R−4sin⁡(δbR(y))δR)∣v(y)∣2 dy. \frac1R\int_{|x|<R}|w|^2\,dx =\frac1{2\pi}\int_{|y|<R} \left(\frac{4b_R(y)}R- \frac{4\sin(\delta b_R(y))}{\delta R}\right)|v(y)|^2\,dy.

The first term tends to 4∥v∥22=44\|v\|_2^2=4 by dominated convergence. The absolute integral of the second is at most 4/(∣δ∣R)4/(|\delta|R). The ball average therefore tends to 2/π2/\pi, and Proposition 2.4 gives dist⁡(w,B0∗)=1/π\operatorname{dist}(w,B^*_0)=1/\sqrt\pi. For n=1n=1, the same calculation uses the scalar slice space and bR=Rb_R=R.

Integral duality from Theorem 1.1 identifies ww with the adjoint action of Tλ−TμT_\lambda-T_\mu on aa. Consequently

∥Tλ−Tμ∥≥∥(Eλ−Eμ)a∥B∗≥dist⁡(w,B0∗)=π−1/2. \|T_\lambda-T_\mu\| \geq\|(E_\lambda-E_\mu)a\|_{B^*} \geq\operatorname{dist}(w,B^*_0)=\pi^{-1/2}.

This uniform separation for distinct energies proves the claim. □\square

The trace theorem extends to rotated affine hyperplanes: the shell norms are invariant under orthogonal rotations, and multiplication by eix⋅ξ0e^{ix\cdot\xi_0} is an isometry. Curvature, or a nonlinear change of Fourier variables, is not accounted for by these two operations.

5. An exact transport resolvent

Consider H0=DtH_0=D_t on L2(Rt×Ryn−1)L^2(\mathbb R_t\times\mathbb R^{n-1}_y), with domain {u:Dtu∈L2}\{u:D_tu\in L^2\}. The earlier Fourier duality proof identifies this domain with the maximal domain of multiplication by the real frequency τ\tau. That multiplication domain is dense: cut off any L2L^2 function to ∣τ∣≤N|\tau|\leq N and use dominated convergence. Multiplication is symmetric there. If vv is in its adjoint domain with value ww, test against every L2L^2 function supported where ∣τ∣≤N|\tau|\leq N. Such functions are in the original domain, and the adjoint identity gives 1∣τ∣≤Nw=τ1∣τ∣≤Nv1_{|\tau|\leq N}w=\tau1_{|\tau|\leq N}v. Monotone convergence gives τv∈L2\tau v\in L^2 and then w=τvw=\tau v. Thus the two domains agree and the operator is self-adjoint. Unitary conjugation gives the stated realization of DtD_t. No spatial boundary is imposed.

Theorem 5.1. For f∈Bf\in B and Im⁡z>0\operatorname{Im}z>0, the Hilbert-space resolvent is

R0(z)f(t,y)=i∫−∞teiz(t−s)f(s,y) ds. R_0(z)f(t,y)=i\int_{-\infty}^t e^{iz(t-s)}f(s,y)\,ds.

For Im⁡z<0\operatorname{Im}z<0, it is

R0(z)f(t,y)=−i∫t∞eiz(t−s)f(s,y) ds. R_0(z)f(t,y)=-i\int_t^{\infty}e^{iz(t-s)}f(s,y)\,ds.

The upper and lower boundary values at every real λ\lambda exist as B∗B^*-valued weak-star limits. They are given by the same integrals with z=λz=\lambda. Their operator norms from BB to B∗B^* are at most two. They satisfy (Dt−λ)u=f(D_t-\lambda)u=f distributionally, and

R0(λ+i0)f−R0(λ−i0)f=i2π eitλFy−1(Tλf). R_0(\lambda+i0)f-R_0(\lambda-i0)f =i\sqrt{2\pi}\,e^{it\lambda} \mathcal F_y^{-1}(T_\lambda f).

Proof. The slice Lt1Ly2L^1_tL^2_y bound makes both integrals well defined and bounds their slice norms by 2∥f∥B\sqrt2\|f\|_B; the exponential has modulus at most one on the respective integration region. Lemma 4.1 gives the B∗B^* bound two. Differentiation for smooth compactly supported ff proves the equation, with (−i)⋅i=1(-i)\cdot i=1 in the upper formula and the analogous lower-endpoint sign in the second. Density in BB proves the distributional equation in general.

For nonreal zz, convolution in tt with the exponential kernel is bounded on L2L^2, since the kernel has L1L^1 norm ∣Im⁡z∣−1|\operatorname{Im}z|^{-1}. Explicitly, the integral triangle inequality followed by weighted Cauchy–Schwarz bounds the squared slice norm by ∥k∥1∫∣k(t−s)∣∥f(s,⋅)∥22ds\|k\|_1\int |k(t-s)|\|f(s,\cdot)\|_2^2ds; integrating in tt gives the squared L2L^2 bound ∥k∥12∥f∥22\|k\|_1^2\|f\|_2^2. Its Fourier multiplier is (τ−z)−1(\tau-z)^{-1}, which identifies it with the Hilbert-space resolvent, including its domain. As z→λz\to\lambda in the relevant half-plane, dominated convergence gives convergence of each slice in Ly2L^2_y. On any bounded ball this gives L2L^2 convergence by the uniform slice bound. To pass to weak-star convergence against g∈Bg\in B, first truncate gg to a ball, and then use the uniform B∗B^* bound to make the pairing with its BB-small tail uniformly small. This proves the asserted topology. Subtracting the two boundary integrals joins them into the full Fourier integral in ss, giving the displayed jump. □\square

6. Radiation, vanishing flux and uniqueness

Define

v+=i∫Re−isλf(s,⋅) ds=i2π Fy−1(Tλf). v_+=i\int_{\mathbb R}e^{-is\lambda}f(s,\cdot)\,ds =i\sqrt{2\pi}\,\mathcal F_y^{-1}(T_\lambda f).

For the upper solution u+=R0(λ+i0)fu_+=R_0(\lambda+i0)f, its slice satisfies

e−itλu+(t,⋅)⟶{0,t→−∞,v+,t→+∞, e^{-it\lambda}u_+(t,\cdot)\longrightarrow \begin{cases}0,&t\to-\infty,\\v_+,&t\to+\infty,\end{cases}

in Ly2L^2_y. These limits follow directly from the tail of the Lt1Ly2L^1_tL^2_y integral. The lower solution has the reversed direction, with limiting amplitude −v+-v_+ at −∞-\infty.

Theorem 6.1. The following conditions on f∈Bf\in B are equivalent:

  1. Tλf=0T_\lambda f=0.
  2. The upper and lower boundary solutions agree.
  3. The upper solution belongs to B0∗B^*_0.
  4. The lower solution belongs to B0∗B^*_0.

Moreover

lim⁡R→∞1R∫∣x∣<R∣u+∣2 dx=∥v+∥22=2π∥Tλf∥22=2Im⁡(u+,f). \lim_{R\to\infty}\frac1R\int_{|x|<R}|u_+|^2\,dx =\|v_+\|_2^2 =2\pi\|T_\lambda f\|_2^2 =2\operatorname{Im}(u_+,f).

Proof. The jump formula proves equivalence of 1 and 2. Approximate u+u_+ by the model w(t,y)=1{t>0}eitλv+(y)w(t,y)=1_{\{t>0\}}e^{it\lambda}v_+(y). Their difference has bounded slice norms tending to zero as t→±∞t\to\pm\infty. For any δ>0\delta>0, choose TT so the slice norm outside [−T,T][-T,T] is at most δ\delta. Its integral over a ball, divided by RR, is bounded by CT/R+2δ2C_T/R+2\delta^2. Therefore u+−w∈B0∗u_+-w\in B^*_0 by Theorem 2.1.

The ball average of ww is

∫∣y∣<R1−∣y∣2/R2 ∣v+(y)∣2 dy, \int_{|y|<R}\sqrt{1-|y|^2/R^2}\,|v_+(y)|^2\,dy,

which tends to ∥v+∥22\|v_+\|_2^2. The cross term between ww and u+−wu_+-w, divided by RR, tends to zero by Cauchy–Schwarz and the vanishing average of the difference. This proves the first limit and equivalence of 1 and 3. The lower solution has the same limiting squared mass, proving 4.

For the last equality put g(t)=e−itλf(t,⋅)g(t)=e^{-it\lambda}f(t,\cdot) and G(t)=∫−∞tg(s) dsG(t)=\int_{-\infty}^tg(s)\,ds. These are Hilbert-valued functions, g∈L1g\in L^1 and GG bounded. The pairing is absolutely integrable, and

Im⁡(u+,f)=Re⁡∫(G(t),g(t))Ly2 dt=12∥G(+∞)∥22. \operatorname{Im}(u_+,f) =\operatorname{Re}\int(G(t),g(t))_{L^2_y}\,dt =\tfrac12\|G(+\infty)\|_2^2.

To justify the second equality directly for every L1L^1 slice forcing, expand ∥∫g∥2=∬(g(s),g(t)) ds dt\|\int g\|^2=\iint(g(s),g(t))\,ds\,dt. The absolute double integral is at most (∫∥g∥)2(\int\|g\|)^2. The diagonal is null, and the two half-planes s<ts<t and s>ts>t give conjugate integrals. Their sum is therefore 2Re⁡∫(G(t),g(t))dt2\operatorname{Re}\int(G(t),g(t))dt. This proves the identity without differentiability of the forcing. Since v+=iG(+∞)v_+=iG(+\infty), the result follows. □\square

Theorem 6.2 (the exact obstruction to norm convergence). For either boundary value u±=R0(λ±i0)fu_\pm=R_0(\lambda\pm i0)f,

dist⁡B∗(u±,B0∗)=π ∥Tλf∥2. \operatorname{dist}_{B^*}(u_\pm,B^*_0) =\sqrt\pi\,\|T_\lambda f\|_2.

Every nonreal zz therefore satisfies

∥R0(z)f−u±∥B∗≥π ∥Tλf∥2. \|R_0(z)f-u_\pm\|_{B^*} \geq\sqrt\pi\,\|T_\lambda f\|_2.

As z→λz\to\lambda in the corresponding half-plane, convergence to u±u_\pm in B∗B^* norm holds if and only if Tλf=0T_\lambda f=0. The approach may change both the real and imaginary parts of zz.

Proof. Theorem 6.1 gives the ball-mass limit 2π∥Tλf∥222\pi\|T_\lambda f\|_2^2 for each sign. Proposition 2.4 gives the distance. Since f∈B⊂L2f\in B\subset L^2, every nonreal Hilbert-space resolvent R0(z)fR_0(z)f lies in L2⊂B0∗L^2\subset B^*_0. The distance consequently bounds its error from below, proving necessity of zero trace.

We prove sufficiency, including arbitrary upper-half-plane approaches. Put g(s)=e−isλf(s,⋅)g(s)=e^{-is\lambda}f(s,\cdot) in the slice Hilbert space H=Ly2\mathcal H=L^2_y, or C\mathbb C when n=1n=1. Lemma 4.1 gives g∈L1(R;H)g\in L^1(\mathbb R;\mathcal H), and zero trace says ∫g=0\int g=0. For h=z−λh=z-\lambda with Im⁡h≥0\operatorname{Im}h\geq0, define

(Khg)(t)=i∫−∞teih(t−s)g(s) ds. (K_hg)(t)=i\int_{-\infty}^t e^{ih(t-s)}g(s)\,ds.

Its norm from L1L^1 to L∞L^\infty is at most one, including h=0h=0. The resolvent and boundary solution are eitλKhge^{it\lambda}K_hg and eitλK0ge^{it\lambda}K_0g.

Choose a scalar ψ∈Cc∞([−1,1])\psi\in C_c^\infty([-1,1]), ψ≥0\psi\geq0, ∫ψ=1\int\psi=1. For M≥1M\geq1 put

gM=1[−M,M]g−ψ∫−MMg(s) ds. g_M=1_{[-M,M]}g-\psi\int_{-M}^M g(s)\,ds.

Then gMg_M is supported in [−M,M][-M,M], its integral is zero, and

∥g−gM∥L1≤2∫∣s∣>M∥g(s)∥H ds⟶0. \|g-g_M\|_{L^1} \leq2\int_{|s|>M}\|g(s)\|_{\mathcal H}\,ds\longrightarrow0.

We need only this slice approximation; gMg_M need not belong to BB. For ℓ≥0\ell\geq0 and Im⁡h≥0\operatorname{Im}h\geq0, integration of the derivative of eihℓe^{ih\ell} gives ∣eihℓ−1∣≤∣h∣ℓ|e^{ih\ell}-1|\leq |h|\ell. When −M≤t≤M-M\leq t\leq M, the upper integral therefore yields

∥(Kh−K0)gM(t)∥H≤2M∣h∣∥gM∥L1. \|(K_h-K_0)g_M(t)\|_{\mathcal H} \leq2M|h|\|g_M\|_{L^1}.

Both integrals vanish for t<−Mt<-M. For t>Mt>M, K0gM=0K_0g_M=0 and cancellation gives

KhgM(t)=ieih(t−M)∫−MM(eih(M−s)−1)gM(s) ds. K_hg_M(t)=i e^{ih(t-M)}\int_{-M}^M (e^{ih(M-s)}-1)g_M(s)\,ds.

The exterior factor has modulus at most one, so the same bound holds there. Thus

∥(Kh−K0)g∥L∞≤2∥g−gM∥L1+2M∣h∣∥gM∥L1. \|(K_h-K_0)g\|_{L^\infty} \leq2\|g-g_M\|_{L^1}+2M|h|\|g_M\|_{L^1}.

First choose MM to make the first term small, and then let h→0h\to0 with that MM fixed. The slice supremum tends to zero, and Lemma 4.1 transfers this convergence to B∗B^*. Reflection t↦−tt\mapsto-t changes the lower integral into an upper integral with parameter −h-h, whose imaginary part is nonnegative. It preserves the zero-integral condition and the norms, so the same proof handles the lower half-plane. □\square

A nonreal transport resolvent loses its tail mass, while its real-energy boundary solution retains it.

For the exact forcing f=1[0,2]f=1_{[0,2]} on the line at energy zero, the boundary amplitude is imin⁡(t,2)i\min(t,2) for t≥0t\geq0, and zero for t<0t<0. The curves sample the exact nonreal solutions at ε=1/2,1/5,1/20\varepsilon=1/2,1/5,1/20. Their ball mass tends to zero, while the boundary ball mass tends to four. The dyadic squared error tends to two, giving the proved norm obstruction 2\sqrt2. The plotted finite-radius values illustrate the analytic limits; they do not establish them.

This criterion has been proved for DtD_t and its explicit transport integral. The general curved and perturbed resolvent lessons specify their boundary topologies separately.

A homogeneous solution u∈B∗u\in B^* of (Dt−λ)u=0(D_t-\lambda)u=0 is eitλv(y)e^{it\lambda}v(y), with v∈Ly2v\in L^2_y. To prove the distributional representation, put U=e−itλuU=e^{-it\lambda}u and choose ρ∈Cc∞(R)\rho\in C_c^\infty(\mathbb R) with ∫ρ=1\int\rho=1. For a compact smooth test φ(t,y)\varphi(t,y), set a(y)=∫φ(t,y)dta(y)=\int\varphi(t,y)dt. The function φ−ρa\varphi-\rho a has zero integral in tt, so its primitive from −∞-\infty is a compactly supported smooth test Ψ(t,y)\Psi(t,y). Since ∂tU=0\partial_tU=0, we have U(φ)=U(ρa)U(\varphi)=U(\rho a). Defining v(a)=U(ρa)v(a)=U(\rho a) proves U=1⊗vU=1\otimes v. Local L2L^2 makes vv a locally square-integrable function by Cauchy–Schwarz applied to ∫ρ(t)U(t,y)dt\int\rho(t)U(t,y)dt. The B∗B^* ball bound, applied to cylinders ∣y∣<L|y|<L, ∣t∣<R/2|t|<R/2 contained in a ball of radius RR for large RR, bounds ∫∣y∣<L∣v∣2\int_{|y|<L}|v|^2 uniformly in LL. Thus v∈L2v\in L^2. Its ball average tends to 2∥v∥22\|v\|^2, so the only homogeneous solution in B0∗B^*_0 is zero. This proves uniqueness in the vanishing-mass class when the Fourier trace vanishes.

3A. Logarithmic forcing at the endpoint

The author-hosted Agmon lectures, recorded by Gustafson and reworked by Taylor, Section 1, compare these spaces with power-weighted Hilbert spaces. A useful refinement is to replace the positive power gap by a logarithm. The following proof uses the shell definitions directly.

Proposition 3.2 (the sharp logarithmic criterion). Give a positive sequence hjh_j, and define the shellwise weight wh(x)=Rj1/2hjw_h(x)=R_j^{1/2}h_j on AjA_j. The two inclusions

L2(wh2 dx)⟶B,B∗⟶L2(wh−2 dx). \begin{gathered} L^2(w_h^2\,dx)\longrightarrow B,\\ B^*\longrightarrow L^2(w_h^{-2}\,dx). \end{gathered}

are bounded if and only if ∑j≥0hj−2<∞\sum_{j\ge0}h_j^{-2}<\infty. In that case their exact norms both equal

Ch=(∑j≥0hj−2)1/2. C_h=\left(\sum_{j\ge0}h_j^{-2}\right)^{1/2}.

In particular, hj=(1+j)βh_j=(1+j)^\beta works exactly when β>1/2\beta>1/2. This gives, with equivalent continuous weights,

⟨x⟩1/2[log⁡(e+∣x∣)]βf∈L2⟹f∈B,u∈B∗⟹⟨x⟩−1/2[log⁡(e+∣x∣)]−βu∈L2. \begin{gathered} \langle x\rangle^{1/2}[\log(e+|x|)]^\beta f\in L^2\\ \Longrightarrow f\in B,\\ u\in B^*\Longrightarrow\\ \langle x\rangle^{-1/2}[\log(e+|x|)]^{-\beta}u\in L^2. \end{gathered}

Proof. Put aj=Rj1/2∥f∥L2(Aj)a_j=R_j^{1/2}\|f\|_{L^2(A_j)}. The first assertion is precisely

∑jaj≤Ch(∑jhj2aj2)1/2, \sum_j a_j\le C_h\left(\sum_j h_j^2a_j^2\right)^{1/2},

which is Cauchy–Schwarz. Its best constant on the first J+1J+1 shells is (∑j=0Jhj−2)1/2(\sum_{j=0}^J h_j^{-2})^{1/2}: take aj=hj−2a_j=h_j^{-2} there and zero elsewhere, and realize the norms with a unit vector ej∈L2(Aj)e_j\in L^2(A_j). Letting JJ increase proves sharpness and necessity. For the second assertion put bj=Rj−1/2∥u∥L2(Aj)b_j=R_j^{-1/2}\|u\|_{L^2(A_j)}; then

∥wh−1u∥22=∑jhj−2bj2≤Ch2∥u∥B∗2. \|w_h^{-1}u\|_2^2=\sum_j h_j^{-2}b_j^2 \le C_h^2\|u\|_{B^*}^2.

The locally square-integrable function u=∑jRj1/2eju=\sum_jR_j^{1/2}e_j has bj=1b_j=1 on every shell, proving the exact constant and failure of the second inclusion when the sum diverges.

For logarithmic weights with β≤1/2\beta\le1/2, failure of the first inclusion also occurs for a single function, not only for unbounded finite-shell constants. Set

aj=(1+j)−β−1/2log⁡(e+j),f=∑j≥1Rj−1/2ajej. a_j=\frac{(1+j)^{-\beta-1/2}}{\log(e+j)},\qquad f=\sum_{j\ge1}R_j^{-1/2}a_je_j.

Its weighted squared norm is ∑j≥1(1+j)−1[log⁡(e+j)]−2<∞\sum_{j\ge1}(1+j)^{-1}[\log(e+j)]^{-2}<\infty, whereas ∑aj\sum a_j diverges for β≤1/2\beta\le1/2, including the harmonic-logarithmic endpoint. Finally ⟨x⟩\langle x\rangle and RjR_j, and log⁡(e+∣x∣)\log(e+|x|) and 1+j1+j, are uniformly comparable on each shell. This proves the continuous-weight version with its equivalence constants. □\square

Corollary 3.3 (weighted observations of an endpoint operator). If T:B→B∗T:B\to B^* is bounded and Ch<∞C_h<\infty, then the operator on ordinary L2L^2 obtained by multiplication on both sides satisfies

∥wh−1Twh−1∥L2→L2≤Ch2∥T∥B→B∗. \|w_h^{-1}T w_h^{-1}\|_{L^2\to L^2} \le C_h^2\|T\|_{B\to B^*}.

Proof. Multiplication by wh−1w_h^{-1} maps L2L^2 into L2(wh2dx)L^2(w_h^2dx), isometrically. Apply the first inclusion, then TT, then the second inclusion. □\square

Thus an already proved endpoint resolvent bound accepts forcing with a logarithmic gap, strictly weaker at infinity than any fixed positive power gap. Explicitly, for every δ>0\delta>0 and real β\beta, (log⁡r)β/rδ→0(\log r)^\beta/r^\delta\to0 as r→∞r\to\infty: for β≤0\beta\leq0 compare with r−δr^{-\delta}, and for β>0\beta>0 put y=δlog⁡ry=\delta\log r and apply the earlier bound yβe−y→0y^\beta e^{-y}\to0. The criterion is exact for arbitrary inputs in the indicated spaces; it does not assert that a particular differential operator fails at a rejected weight. At the further borderline hj=(1+j)1/2[log⁡(e+j)]γh_j=(1+j)^{1/2}[\log(e+j)]^\gamma, the same proof gives the exact criterion γ>1/2\gamma>1/2. The integral test proves this by the substitution s=log⁡ts=\log t in ∫dt/(t(log⁡t)2γ)\int dt/(t(\log t)^{2\gamma}).

Agmon's Proposition 1.A transfers two Hilbert operator bounds to the shell spaces. The following direct proof uses an unweighted bound and only one weighted bound. The stronger two-sided, general adjacent-weight theorem in Mild weights and frequency localization, Theorem 2.1, remains available for other weights.

Proposition 3.4 (one weighted endpoint suffices). Suppose TT is bounded on L2L^2 and its restriction is bounded on L12L^2_1, with norms M0,M1M_0,M_1, respectively. Then T:B→BT:B\to B is bounded, with

∥T∥B→B≤M0+3θM11−θ,θ=2−1/2. \|T\|_{B\to B}\le\frac{M_0+3\theta M_1}{1-\theta}, \qquad\theta=2^{-1/2}.

If instead it has consistent bounds on L2L^2 and L−12L^2_{-1}, the corresponding estimate holds on B∗B^*, and TT preserves B0∗B^*_0.

Proof. On AjA_j the continuous weight ⟨x⟩\langle x\rangle lies between Rj/2R_j/2 and 2Rj\sqrt2 R_j, also for j=0j=0. The two operator bounds therefore give

∥1AjT1Ak∥2→2≤min⁡(M0,3M1RkRj). \|\mathbf1_{A_j}T\mathbf1_{A_k}\|_{2\to2} \le\min\left(M_0,3M_1\frac{R_k}{R_j}\right).

For a finite shell input set ak=Rk1/2∥f∥L2(Ak)a_k=R_k^{1/2}\|f\|_{L^2(A_k)}. Multiplying the block estimate by the output shell weight yields

Rj1/2∥Tf∥L2(Aj)≤∑k≥jM0θk−jak+∑k<j3M1θj−kak. R_j^{1/2}\|Tf\|_{L^2(A_j)} \le \sum_{k\ge j}M_0\theta^{k-j}a_k +\sum_{k<j}3M_1\theta^{j-k}a_k.

Sum in jj. The first geometric sum, including its zero term, is M0/(1−θ)M_0/(1-\theta), and the second is 3M1θ/(1−θ)3M_1\theta/(1-\theta). This proves the asserted constant. Finite shell inputs converge in BB, and hence in L2L^2; the bounded BB-extension therefore agrees with the original L2L^2 operator.

For the second assertion, the L2L^2 adjoint T∗T^* has the same unweighted bound and a bound on L12L^2_1 with norm at most the given L−12L^2_{-1} norm. Indeed let SS denote the consistent bounded action on L−12L^2_{-1}, and let M−1M_{-1} be its norm. For g∈L12g\in L^2_1, the functional f↦(Sf,g)f\mapsto(Sf,g) on L−12L^2_{-1} has norm at most M−1∥g∥L12M_{-1}\|g\|_{L^2_1}. The weighted duality proved in the first spectral lesson represents it by a vector v∈L12v\in L^2_1 with this norm bound. For compactly supported L2L^2 tests ff, consistency and the ordinary adjoint give (f,v)=(Tf,g)=(f,T∗g)(f,v)=(Tf,g)=(f,T^*g). Their L2L^2 density proves v=T∗gv=T^*g, which is precisely the claimed weighted bound. Apply the first part to T∗T^*, then use the exact BB-duality in Theorem 1.1. This defines the bounded action of TT on B∗B^*. It agrees with the given weighted operator: shell truncations of a B∗B^* input converge in L−12L^2_{-1}, since the squared tail is at most C∥u∥B∗2∑j>J2−jC\|u\|_{B^*}^2\sum_{j>J}2^{-j}, and pairings against BB converge by the shell sum. To make the identification explicit, write the dual action as (f,T~u)=(T∗f,u)(f,\widetilde Tu)=(T^*f,u), f∈Bf\in B. For a compactly supported smooth ff, the truncated inputs uJu_J give (SuJ,f)=(uJ,T∗f)(Su_J,f)=(u_J,T^*f). The left side converges to (Su,f)(Su,f) by weighted duality, and the right side to (u,T∗f)=(T~u,f)(u,T^*f)=(\widetilde Tu,f) by the BB shell tail of T∗fT^*f. Thus the two locally square-integrable functions agree as distributions and hence almost everywhere, by compact smooth test density on each bounded region. Finally approximate an input in B0∗B^*_0 in that norm by compactly supported L2L^2 inputs, using Theorem 2.1. Their images are in L2⊂B0∗L^2\subset B^*_0, and this subspace is closed. □\square

Use the conclusion

Use Proposition 2.4 and Theorem 6.2 to separate distance from the vanishing-tail subspace, weak-star convergence and norm convergence. A nonzero shell trace must remain visible in that comparison.

7. Exercises

Exercise 7.1 (foundation). For u(x)=1{∣x∣≥1}∣x∣−n/2u(x)=1_{\{|x|\geq1\}}|x|^{-n/2}, decide membership in L2L^2, B∗B^* and B0∗B^*_0.

Exercise 7.2 (foundation). On the line, take f(t)=eiλt1[0,2](t)f(t)=e^{i\lambda t}1_{[0,2]}(t). Compute both resolvent boundary solutions, their mass per unit radius, and their exact distance to B0∗B^*_0. What lower bound does this give for the error of every nonreal resolvent?

Exercise 7.3 (intermediate). Construct a nonzero compactly supported forcing term on the line for which the two boundary solutions agree. Compute that common solution explicitly and prove norm convergence of both nonreal resolvents to it.

Exercise 7.4 (intermediate). Prove that fk→ff_k\to f in BB implies Tλfk→TλfT_\lambda f_k\to T_\lambda f uniformly for λ∈R\lambda\in\mathbb R. Use the exact extension mass to prove the quantitative failure of continuity of TλT_\lambda in operator norm.

Exercise 7.5 (advanced). Let Dv=−iv⋅∇D_v=-iv\cdot\nabla, v≠0v\ne0. By rotation and rescaling of the transport equation, derive the boundary formula and the outgoing mass identity. Retain the factor ∣v∣|v|.

8. Complete solutions

Solution 7.1. The squared radial integral is ∣Sn−1∣∫1Rr−1 dr=∣Sn−1∣log⁡R|\mathbb S^{n-1}|\int_1^Rr^{-1}\,dr=|\mathbb S^{n-1}|\log R. It diverges, so u∉L2u\notin L^2. Dividing by RR gives a bounded quantity tending to zero, so Theorem 2.1 places uu in B0∗B^*_0, and hence in B∗B^*. Vanishing mass per radius is weaker than square integrability.

Solution 7.2. The upper solution is ieiλtie^{i\lambda t} times 00, tt, or 22, according as t<0t<0, 0≤t≤20\leq t\leq2, or t>2t>2. The lower solution is −ieiλt-ie^{i\lambda t} times 22, 2−t2-t, or 00 on those same regions. Their difference is 2ieiλt2ie^{i\lambda t}. Each squared mass on [−R,R][-R,R], divided by RR, tends to four. The outgoing amplitude is 2i2i; its squared modulus is four, agreeing with Theorem 6.1. Proposition 2.4 gives distance 4/2=2\sqrt{4/2}=\sqrt2 for each boundary solution. Every nonreal resolvent lies in B0∗B^*_0, so its error from either boundary solution is at least 2\sqrt2, regardless of how near its parameter is to λ\lambda.

Solution 7.3. Put f(t)=eiλt(1[0,1](t)−1[1,2](t))f(t)=e^{i\lambda t}(1_{[0,1]}(t)-1_{[1,2]}(t)). The integral of e−iλtf(t)e^{-i\lambda t}f(t) is zero. The common solution is ieiλtie^{i\lambda t} times 00 for t<0t<0, tt for 0≤t≤10\leq t\leq1, 2−t2-t for 1≤t≤21\leq t\leq2, and 00 for t>2t>2. It is compactly supported and belongs to L2L^2. Its distributional derivative gives the forcing without delta terms, because it is continuous at all three joining points. For a direct norm estimate, g=e−itλfg=e^{-it\lambda}f has integral zero, support in [0,2][0,2] and L1L^1 norm two. The proof of Theorem 6.2 gives ∥(Kh−K0)g∥L∞≤4∣h∣\|(K_h-K_0)g\|_{L^\infty}\leq4|h|: on [0,2][0,2] the integration interval has length at most two; after two use the zero integral and factor out eih(t−2)e^{ih(t-2)}. Before zero both upper integrals vanish. Hence the upper B∗B^* error is at most 42∣z−λ∣4\sqrt2|z-\lambda|. Reflection gives the same estimate for the lower solution. Both errors tend to zero.

Solution 7.4. The trace bound gives sup⁡λ∥Tλ(fk−f)∥2≤π−1/2∥fk−f∥B→0\sup_\lambda\|T_\lambda(f_k-f)\|_2\leq\pi^{-1/2}\|f_k-f\|_B\to0. For distinct λ,μ\lambda,\mu, test the adjoint difference on a unit amplitude aa. Its extension is (2π)−1/2(eitλ−eitμ)Fy−1a(2\pi)^{-1/2}(e^{it\lambda}-e^{it\mu})\mathcal F_y^{-1}a. Integrating in tt over the ball gives the formula in Proposition 4.3: the constant term has limit 2/π2/\pi, and the oscillatory term is bounded by 2/(π∣λ−μ∣R)2/(\pi|\lambda-\mu|R), which tends to zero. Its exact distance to B0∗B^*_0 is therefore 1/π1/\sqrt\pi. Integral duality yields ∥Tλ−Tμ∥≥1/π\|T_\lambda-T_\mu\|\geq1/\sqrt\pi. Strong continuity fixes one forcing term; the operator norm ranges over all unit forcing terms, whose tail cutoffs need not be uniform.

Solution 7.5. Choose coordinates x=tv^+yx=t\widehat v+y, v^=v/∣v∣\widehat v=v/|v|, y⊥vy\perp v. Then Dv=∣v∣DtD_v=|v|D_t, and

(Dv−λ−i0)−1f=i∣v∣∫−∞teiλ(t−s)/∣v∣f(s,y) ds. (D_v-\lambda-i0)^{-1}f =\frac{i}{|v|}\int_{-\infty}^t e^{i\lambda(t-s)/|v|}f(s,y)\,ds.

The outgoing amplitude is a=i∣v∣−1∫e−iλs/∣v∣f(s,⋅) dsa=i|v|^{-1}\int e^{-i\lambda s/|v|}f(s,\cdot)\,ds. The ball-average argument is unchanged by the rotation, giving limit ∥a∥2\|a\|^2. The flux calculation instead gives 2Im⁡(u,f)=∣v∣∥a∥22\operatorname{Im}(u,f)=|v|\|a\|^2, since the equation has coefficient ∣v∣|v| before DtD_t. Hence the mass limit is 2∣v∣−1Im⁡(u,f)2|v|^{-1}\operatorname{Im}(u,f). This also follows from u=∣v∣−1R0(λ/∣v∣+i0)fu=|v|^{-1}R_0(\lambda/|v|+i0)f. Dropping the speed would confuse a spatial mass with an energy flux.

References