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Positive energy and vanishing at the far end of space

Decay at infinity can be tested by weights that grow as increasingly high powers of the radius. For a positive-energy equation, the useful estimate must control two scales at once: the power in the weight and the radius at which the solution is being tested. Their competition creates a characteristic frequency shell. An estimate that ignores that shell loses the second derivatives needed to handle rough leading coefficients.

We organize the argument around two complementary estimates. A Fourier calculation, localized on the sphere, recovers derivatives with carefully chosen radius-dependent coefficients. A difference of squared norms supplies the angular and positive-energy terms. Neither estimate closes by itself. Their combination makes the coefficient errors small and gives a weighted uniqueness theorem for complex Lipschitz perturbations of a real elliptic quadratic operator.

1. The exterior equation and its precise assumptions

Let X⊂ℝnX\subset\mathbb R^n, n≥1n\geq1, be a connected open neighborhood of infinity: {|x|>R*}⊂X\{|x|>R_*\}\subset X for some R*R_*. Let p(x,D)=∑j,k=1najk(x)DjDk,Dj=−i∂xj.(E1) p(x,D)=\sum_{j,k=1}^n a_{jk}(x)D_jD_k, \qquad D_j=-i\partial_{x_j}. \tag{E1} The coefficients may be complex. They are locally Lipschitz on XX, and their symmetric part is elliptic on XX: ∑j,kajk(x)ξjξk≠0(x∈X,ξ∈ℝn\0).(E2) \sum_{j,k}a_{jk}(x)\xi_j\xi_k\ne0 \quad(x\in X,\ \xi\in\mathbb R^n\setminus0). \tag{E2} Assume that for some δ>0\delta>0, some CaC_a, and all sufficiently large |x||x|, |ajk(x)−δjk|≤Ca|x|−1−δ,|∇ajk(x)|≤Ca|x|−2−δa.e.(E3) |a_{jk}(x)-\delta_{jk}|\leq C_a|x|^{-1-\delta}, \qquad |\nabla a_{jk}(x)|\leq C_a|x|^{-2-\delta} \quad\text{a.e.} \tag{E3} The two powers in (E3) are distinct. No second derivative of a leading coefficient is assumed. Retain the full matrix, including its skew part. Put as=(a+aT)/2a^s=(a+a^T)/2 and aa=(a−aT)/2a^a=(a-a^T)/2. The exact comparison is ∑j,kajka(x)DjDk=∑j<kajk(x)−akj(x)2(DjDk−DkDj)=0.(E2a) \sum_{j,k}a^a_{jk}(x)D_jD_k =\sum_{j<k}\frac{a_{jk}(x)-a_{kj}(x)}2 (D_jD_k-D_kD_j)=0. \tag{E2a} Both derivatives remain to the right of the coefficient. Thus no derivative of a skew coefficient is introduced. Formula (E2a) proves that contribution is zero; it does not erase the original entries from the coefficient data.

Here is the complete formulation for an original real limiting matrix A∞A_\infty, which need not be symmetric. Replace the first assumption in (E3) by |ajk(x)−(A∞)jk|≤Ca|x|−1−δ,|∇ajk(x)|≤Ca|x|−2−δ.(E3a) |a_{jk}(x)-(A_\infty)_{jk}|\leq C_a|x|^{-1-\delta}, \qquad |\nabla a_{jk}(x)|\leq C_a|x|^{-2-\delta}. \tag{E3a} Assume its real symmetric part is definite. Choose its actual sign σ∈{1,−1}\sigma\in\{1,-1\}, and set A∞s=(A∞+A∞T)/2,A∞a=(A∞−A∞T)/2,G=σA∞s>0,M=G1/2,Y=M−1X,v(y)=u(My),ã(y)=σM−1a(My)M−T,p̃=∑j,kãjk(y)DyjDyk,λ̃=σλ,K∞=σM−1A∞aM−T,ã(∞)=I+K∞,K∞T=−K∞.(E3b) \begin{gathered} A_\infty^s=(A_\infty+A_\infty^T)/2,\qquad A_\infty^a=(A_\infty-A_\infty^T)/2,\\ G=\sigma A_\infty^s>0,\qquad M=G^{1/2},\qquad Y=M^{-1}X,\qquad v(y)=u(My),\\ \widetilde a(y)=\sigma M^{-1}a(My)M^{-T},\quad \widetilde p=\sum_{j,k}\widetilde a_{jk}(y)D_{y_j}D_{y_k},\quad \widetilde\lambda=\sigma\lambda,\\ K_\infty=\sigma M^{-1}A_\infty^aM^{-T},\qquad \widetilde a(\infty)=I+K_\infty,\qquad K_\infty^T=-K_\infty. \end{gathered} \tag{E3b} The original A∞,a,p,u,X,λA_\infty,a,p,u,X,\lambda remain fixed. The auxiliary limit is the full I+K∞I+K_\infty, with every skew entry retained. The theorem below holds in this formulation when σλ>0\sigma\lambda>0. For the identity limit, σ=1\sigma=1, M=IM=I, and K∞=0K_\infty=0.

We prove every map needed to apply the exterior argument. The chain rule and its inverse give Dyv(y)=MTDxu(My),Dxu(My)=M−TDyv(y),((p̃−λ̃)v)(y)=σ((p−λ)u)(My),∂ylãjk(y)=σ∑r,s,h(M−1)jr(M−1)ksMhl(∂xhars)(My).(E3c) \begin{gathered} D_yv(y)=M^TD_xu(My),\qquad D_xu(My)=M^{-T}D_yv(y),\\ ((\widetilde p-\widetilde\lambda)v)(y) =\sigma((p-\lambda)u)(My),\\ \partial_{y_l}\widetilde a_{jk}(y) =\sigma\sum_{r,s,h}(M^{-1})_{jr}(M^{-1})_{ks}M_{hl} (\partial_{x_h}a_{rs})(My). \end{gathered} \tag{E3c} The derivative identity holds almost everywhere. Constant linear pullback and its inverse map Hlock(X)H^k_{\mathrm{loc}}(X) bijectively to Hlock(Y)H^k_{\mathrm{loc}}(Y), k=0,1,2k=0,1,2: every weak derivative is the finite chain-rule sum, and changing variables contributes |det⁡M|−1|\det M|^{-1} to its squared norm. Smooth approximation proves these identities at weak regularity. The distributional identity in (E3c) then follows for the weak Lipschitz coefficient product as well; it agrees with the usual expression when the local regularity has reached H2H^2.

Let m−m_- and m+m_+ be the smallest and largest singular values of MM. Then 0<m−≤m+0<m_-\leq m_+ and m−|y|≤|My|≤m+|y|m_-|y|\leq|My|\leq m_+|y|. Assumption (E3a) and the full sums in (E3c) imply, entry by entry, |ãjk(y)−δjk−(K∞)jk|≤Cam−−1−δ|y|−1−δ∑r,s|(M−1)jr(M−1)ks|,|∂ylãjk(y)|≤Cam−−2−δ|y|−2−δ∑r,s,h|(M−1)jr(M−1)ksMhl|.(E3d) \begin{split} |\widetilde a_{jk}(y)-\delta_{jk}-(K_\infty)_{jk}| &\leq C_a m_-^{-1-\delta}|y|^{-1-\delta} \sum_{r,s}|(M^{-1})_{jr}(M^{-1})_{ks}|,\\ |\partial_{y_l}\widetilde a_{jk}(y)| &\leq C_a m_-^{-2-\delta}|y|^{-2-\delta} \sum_{r,s,h}|(M^{-1})_{jr}(M^{-1})_{ks}M_{hl}|. \end{split} \tag{E3d} The image domain contains {|y|>R*/m−}\{|y|>R_*/m_-\}. For the original inequality (E5), its complete pullback is |(p̃−λ̃)v(y)|≤C|My|−1(|v(y)|+|M−TDyv(y)|).(E3e) |(\widetilde p-\widetilde\lambda)v(y)| \leq C|My|^{-1}\bigl(|v(y)|+|M^{-T}D_yv(y)|\bigr). \tag{E3e} In particular it has the required |y|−1|y|^{-1} bound with the explicit additional constant m−−1max⁡(1,m−−1)m_-^{-1}\max(1,m_-^{-1}). The original form of (E3e) is retained when returning the estimate to xx.

Put ℓ−=min⁡(1,m−)\ell_- =\min(1,m_-) and ℓ+=max⁡(1,m+)\ell_+=\max(1,m_+). For every real exponent ss, min⁡(ℓ−s,ℓ+s)(1+|y|)s≤(1+|My|)s≤max⁡(ℓ−s,ℓ+s)(1+|y|)s,∫Y(1+|My|)2s(|v|2+|M−TDyv|2)dy=|det⁡M|−1∫X(1+|x|)2s(|u|2+|Dxu|2)dx.(E3f) \begin{gathered} \min(\ell_-^s,\ell_+^s)(1+|y|)^s \leq(1+|My|)^s \leq\max(\ell_-^s,\ell_+^s)(1+|y|)^s,\\ \int_Y(1+|My|)^{2s} \bigl(|v|^2+|M^{-T}D_yv|^2\bigr)\,dy =|\det M|^{-1}\int_X(1+|x|)^{2s} \bigl(|u|^2+|D_xu|^2\bigr)\,dx. \end{gathered} \tag{E3f} The bounds on M−TM^{-T}, together with (E3f), prove both directions of the all-weight condition (E4), including negative exponents. Ellipticity is also preserved exactly: the auxiliary symbol at a real covector ξ\xi is σpMy(M−Tξ)\sigma p_{My}(M^{-T}\xi), and M−Tξ≠0M^{-T}\xi\ne0 for ξ≠0\xi\ne0. Equations (E2a) and (E8a) below account for the entire skew operator. Sections 2–12 prove the estimate for the auxiliary expression with these original data present, and (E77)–(E80) return it with its full Jacobian to the original operator. A negative-definite limiting form requires the original λ<0\lambda<0, since the positive potential is λ̃=σλ\widetilde\lambda=\sigma\lambda. The example in Section 13 shows why that sign cannot be omitted.

Exterior uniqueness theorem. Suppose λ>0\lambda>0, u∈Hloc1(X)u\in H^1_{\mathrm{loc}}(X), and (1+|x|)sDαu∈L2(X)for every real s and |α|≤1.(E4) (1+|x|)^s D^\alpha u\in L^2(X) \quad\text{for every real }s\text{ and }|\alpha|\leq1. \tag{E4} Suppose the distribution (p−λ)u(p-\lambda)u has a locally square-integrable representative away from the origin and satisfies |(p−λ)u|≤C|x|−1(|u|+|Du|)a.e. on X\{0}.(E5) |(p-\lambda)u|\leq C|x|^{-1}(|u|+|Du|) \quad\text{a.e. on }X\setminus\{0\}. \tag{E5} Then u=0u=0 almost everywhere on XX.

The same conclusion holds if the estimate (E5) is imposed only near infinity and |pu|≤CK(|u|+|Du|)|pu|\leq C_K(|u|+|Du|) is assumed on each compact subset of X\{0}X\setminus\{0\}. The exterior proof uses (E5); propagation through bounded regions uses that local inequality. This more local sufficient formulation does not assert one global constant in bounded regions approaching a finite boundary of XX. If the displayed equation is imposed on all of XX, (E5) already supplies the local inequality on every such compact set. A value at the single point zero has no effect on an H1H^1 function as an almost-everywhere equivalence class.

Ellipticity on the whole continuation domain is explicit in (E2). The decay assumptions alone guarantee it sufficiently far out, since Re⁡∑ajkξjξk≥|ξ|2/2\operatorname{Re}\sum a_{jk}\xi_j\xi_k\geq |\xi|^2/2 there. They give no ellipticity guarantee in an arbitrary bounded part added to XX. If only the exterior conditions are known, the conclusion proved below is vanishing on a sufficiently distant exterior region; the extension across a larger connected domain requires (E2) and the local equation there. This makes explicit the elliptic setting of the antecedent theorem.

The following prerequisites specify the current proof boundary.

We use the stated predecessor results and prove the exterior estimate below.

For the proof choose once and for all 0<d<min⁡(δ,1),0<η<d.(E6) 0<d<\min(\delta,1),\qquad 0<\eta<d. \tag{E6} The original condition (E3) implies the same bounds with dd in place of δ\delta when |x|≥1|x|\geq1. Thus using d<1d<1 in an estimate imposes no extra restriction on the theorem. The number η\eta controls the curvature of the weight. All constants may depend on these two fixed numbers and on λ,n,Ca\lambda,n,C_a, but never on the subsequently large parameters T0T_0 and τ\tau.

2. A cylindrical operator with a growing potential

Set x=etωx=e^t\omega, ω∈Sn−1\omega\in S^{n-1}, and Z(t,ω)=u(etω)Z(t,\omega)=u(e^t\omega). Write Ωj\Omega_j for the projection of eje_j onto the tangent space of the unit sphere. The identities in Section 3 of Detecting a solution from infinite-order silence at one point are ∂xj=e−t(ωj∂t+Ωj),Ωjωk=δjk−ωjωk,∑jωjΩj=0,Ωj*=−Ωj+(n−1)ωj,ΔS=∑jΩj2,−⟨ΔSv,v⟩=∑j∥Ωjv∥2.(E7) \begin{gathered} \partial_{x_j}=e^{-t}(\omega_j\partial_t+\Omega_j),\qquad \Omega_j\omega_k=\delta_{jk}-\omega_j\omega_k,\qquad \sum_j\omega_j\Omega_j=0,\\ \Omega_j^*=-\Omega_j+(n-1)\omega_j,\qquad \Delta_S=\sum_j\Omega_j^2, \qquad -\langle\Delta_Sv,v\rangle=\sum_j\|\Omega_jv\|^2. \end{gathered} \tag{E7} The last two formulas use surface measure. Individual Ωj\Omega_j are not skew adjoint. Their divergence corrections cancel in the sum of squares because ∑ωjΩj=0\sum\omega_j\Omega_j=0.

Twice applying the first identity, with the derivative of e−te^{-t} retained, gives −e2tpu=∑j,kajk(etω)(ωj∂t−ωj+Ωj)(ωk∂t+Ωk)Z.(E8) -e^{2t}pu= \sum_{j,k}a_{jk}(e^t\omega) (\omega_j\partial_t-\omega_j+\Omega_j) (\omega_k\partial_t+\Omega_k)Z. \tag{E8} There is no derivative of ajka_{jk} in this formula: (E1) has coefficients to the left of the derivatives. When ajk=δjka_{jk}=\delta_{jk}, expand (E8) and use (E7) to obtain ∂t2+(n−2)∂t+ΔS.(E9) \partial_t^2+(n-2)\partial_t+\Delta_S. \tag{E9} For the full comparison (E3b), apply this calculation to y=etωy=e^t\omega and v(y)v(y), so the original point is x=etMωx=e^tM\omega. Write ã=I+K∞+r̃\widetilde a=I+K_\infty+\widetilde r, retaining each of its three contributions. The exact frozen skew contribution is ∑j,k(K∞)jk(ωj∂t−ωj+Ωj)(ωk∂t+Ωk)=e2t∑j,k(K∞)jk∂yj∂yk=0.(E8a) \begin{split} &\sum_{j,k}(K_\infty)_{jk} (\omega_j\partial_t-\omega_j+\Omega_j) (\omega_k\partial_t+\Omega_k)\\ &\qquad=e^{2t}\sum_{j,k}(K_\infty)_{jk} \partial_{y_j}\partial_{y_k}=0. \end{split} \tag{E8a} The equality follows from twice applying the full polar formula (E7). Pairing indices in the last sum proves zero because the second derivatives commute and K∞K_\infty is skew. The surviving expression is (E9) plus every term from r̃\widetilde r; (E3d) gives its two required decay bounds. In all subsequent formulas for this case, U(T,ω)=u(et(T)Mω)U(T,\omega)=u(e^{t(T)}M\omega), the coefficient error comes from the complete r̃\widetilde r, and the positive potential uses λ̃=σλ\widetilde\lambda=\sigma\lambda. No original matrix entry or sign has been silently replaced.

Every other coefficient in this cylindrical expression, together with its first cylindrical derivatives, is O(e−(1+d)t)O(e^{-(1+d)t}). An angular or tt derivative of a(etω)a(e^t\omega) introduces one factor ete^t, exactly balancing one power in the derivative bound of (E3). Derivatives of the smooth sphere factors are bounded.

Now introduce the increasing coordinate t=T−e−ηT,h(T)=dtdT=1+ηe−ηT.(E10) t=T-e^{-\eta T},\qquad h(T)=\frac{dt}{dT}=1+\eta e^{-\eta T}. \tag{E10} For T>0T>0, |T−t|<1|T-t|<1, and hh and h−1h^{-1} are uniformly bounded. Put U(T,ω)=Z(t(T),ω)U(T,\omega)=Z(t(T),\omega). Multiply the operator in (E8), with the term λe2t\lambda e^{2t} added, by h2h^2. It becomes Q=∂T2+c(T)∂T+a(T)ΔS+B+Λ(T),B=∑j+|α|≤2bαj(T,ω)∂TjΩα,(E11) Q=\partial_T^2+c(T)\partial_T+a(T)\Delta_S+B+\Lambda(T), \quad B=\sum_{j+|\alpha|\leq2}b_{\alpha j}(T,\omega) \partial_T^j\Omega^\alpha, \tag{E11} where a(T)=h(T)2,c(T)=(n−2)h(T)+η2e−ηTh(T),Λ(T)=λe2Te−2e−ηTh(T)2,|bαj|+|∂Tbαj|+∑l|Ωlbαj|≤Ce−(1+d)T.(E12) \begin{split} a(T)&=h(T)^2,\\ c(T)&=(n-2)h(T)+\frac{\eta^2e^{-\eta T}}{h(T)},\\ \Lambda(T)&=\lambda e^{2T}e^{-2e^{-\eta T}}h(T)^2,\\ |b_{\alpha j}|+|\partial_Tb_{\alpha j}|+ \sum_l|\Omega_lb_{\alpha j}|&\leq C e^{-(1+d)T}. \end{split} \tag{E12} Here Ωα\Omega^\alpha denotes a fixed ordered word; we may sum over all words of the specified length. Indeed h2∂t2=∂T2−(h′/h)∂Th^2\partial_t^2=\partial_T^2-(h'/h)\partial_T, with h′=−η2e−ηTh'=-\eta^2e^{-\eta T}, which proves the formula for cc. Smooth factors involving h,h−1,h′h,h^{-1},h' preserve the last bound of (E12), including its weak first derivatives.

The potential is retained as a main term. Direct differentiation gives Λ′Λ=2+2ηe−ηT−2η2e−ηTh(T)→2,Λ≍λe2T,Λ′≥λe2T(E13) \frac{\Lambda'}{\Lambda} =2+2\eta e^{-\eta T} -\frac{2\eta^2e^{-\eta T}}{h(T)}\longrightarrow2, \quad \Lambda\asymp\lambda e^{2T},\quad \Lambda'\geq\lambda e^{2T} \tag{E13} after increasing a fixed lower threshold for TT. The sign λ>0\lambda>0 is used here.

In these coordinates the differential inequality becomes |QU|≤C(eT|U|+|∂TU|+∑j|ΩjU|).(E14) |QU|\leq C\left(e^T|U|+|\partial_TU|+ \sum_j|\Omega_jU|\right). \tag{E14} To check the powers, before changing tt, multiplication of (E5) by e2te^{2t} gives a zeroth-order term et|Z|e^t|Z| and first-order terms |(ωj∂t+Ωj)Z||(\omega_j\partial_t+\Omega_j)Z|. The bounded factors in (E10) then give (E14). The norm convention on the cylinder is dTdωdT\,d\omega; it is not Euclidean measure. The latter is dx=ent(T)h(T)dTdω.(E15) dx=e^{nt(T)}h(T)\,dT\,d\omega. \tag{E15}

For τ≥1\tau\geq1, write V=eτTU,Qτ=eτTQe−τT.(E16) V=e^{\tau T}U,\qquad Q_\tau=e^{\tau T}Qe^{-\tau T}. \tag{E16} Thus every ∂T\partial_T in (E11) is replaced by ∂T−τ\partial_T-\tau, whereas angular derivatives are unchanged. Our target is τ2∥V∥2+∥∂TV∥2+∑j∥ΩjV∥2+∥eTV∥2≤C(e−T0/2+τ−1)∥QτV∥2(E17) \tau^2\|V\|^2+\|\partial_TV\|^2+ \sum_j\|\Omega_jV\|^2+\|e^TV\|^2 \leq C\left(e^{-T_0/2}+\tau^{-1}\right)\|Q_\tau V\|^2 \tag{E17} for compactly supported smooth VV in (T0,∞)×Sn−1(T_0,\infty)\times S^{n-1}. Since (τ+eT)2(\tau+e^T)^2 is comparable to τ2+e2T\tau^2+e^{2T}, this is also the estimate with weight (τ+eT)1−k(\tau+e^T)^{1-k} on each derivative of order k≤1k\leq1.

3. The error budget and one-derivative algebra

Let 𝒟kV\mathcal D^k V denote the finite family of all words of length kk in ∂T,Ω1,…,Ωn\partial_T,\Omega_1,\ldots,\Omega_n. A squared norm of this family means the sum of the squared norms of its members; 𝒟0V=V\mathcal D^0V=V. On a fixed sphere chart these norms through order two are equivalent to coordinate Sobolev norms, with lower orders included. Define W(V)=τ−1∥e−T𝒟2V∥2+∥𝒟1V∥2+τ2∥V∥2,F(V)=τ3∥e−ηT/2V∥2,R(V)=W(V)+τ3∥e−dTV∥2+τ∥e−dT𝒟1V∥2.(E18) \begin{split} W(V)&=\tau^{-1}\|e^{-T}\mathcal D^2V\|^2 +\|\mathcal D^1V\|^2+\tau^2\|V\|^2,\\ F(V)&=\tau^3\|e^{-\eta T/2}V\|^2,\\ R(V)&=W(V)+\tau^3\|e^{-dT}V\|^2 +\tau\|e^{-dT}\mathcal D^1V\|^2. \end{split} \tag{E18} The highest-order term uses exactly order two; it carries both e−Te^{-T} and τ−1\tau^{-1}. We will not replace it by an unweighted lower-order error.

Two elementary product estimates explain this choice. Consider a term I=∫e−(1+d)Tτj|𝒟rV||𝒟sV|dTdω,j+r+s≤3,r,s≤2,j≥0.(E19) I=\int e^{-(1+d)T}\tau^j |\mathcal D^rV|\,|\mathcal D^sV|\,dT\,d\omega, \quad j+r+s\leq3,\quad r,s\leq2,\quad j\geq0. \tag{E19} All the indices here are nonnegative integers. If r=2r=2, then j+s≤1j+s\leq1, and the integrand is the product (τ−1/2e−T|𝒟2V|)(τj+1/2e−dT|𝒟sV|).(E20) \left(\tau^{-1/2}e^{-T}|\mathcal D^2V|\right) \left(\tau^{j+1/2}e^{-dT}|\mathcal D^sV|\right). \tag{E20} The square of the second factor is bounded by the order-ss term in the decaying part of RR, because 2j+1≤3−2s2j+1\leq3-2s. Cauchy–Schwarz and 2ab≤a2+b22ab\leq a^2+b^2 bound (E19) by CRCR. The case s=2s=2 is identical with the two factors reversed. If r,s≤1r,s\leq1, use d<1d<1, hence e−(1+d)T≤e−2dTe^{-(1+d)T}\leq e^{-2dT} for T>0T>0, and j≤3−r−sj\leq3-r-s. The product of τ3/2−re−dT|𝒟rV|\tau^{3/2-r}e^{-dT}|\mathcal D^rV| and τ3/2−se−dT|𝒟sV|\tau^{3/2-s}e^{-dT}|\mathcal D^sV| dominates the integrand. Their squares again occur in RR. This proves a uniform bound for every monomial in (E19), not just a representative highest-order term.

We also need products containing the potential. If kk and its first derivatives are O(e−(1+d)T)O(e^{-(1+d)T}), then |Λk|+|∂T(Λk)|+∑l|Ωl(Λk)|≤Ce(1−d)T.(E21) |\Lambda k|+|\partial_T(\Lambda k)|+ \sum_l|\Omega_l(\Lambda k)| \leq C e^{(1-d)T}. \tag{E21} Consequently, for every fixed θ>0\theta>0, C∫e(1−d)T(τ|V|2+|𝒟1V||V|)≤θ∥eTV∥2+Cθ(τ2∥V∥2+∥𝒟1V∥2).(E22) \begin{split} C\int e^{(1-d)T} \left(\tau|V|^2+|\mathcal D^1V|\,|V|\right) &\leq \theta\|e^TV\|^2 +C_\theta\left(\tau^2\|V\|^2+\|\mathcal D^1V\|^2\right). \end{split} \tag{E22} For the first integrand apply Young’s inequality to eT|V|e^T|V| and τe−dT|V|\tau e^{-dT}|V|; for the second use eT|V|e^T|V| and e−dT|𝒟1V|e^{-dT}|\mathcal D^1V|. The factors e−dT≤1e^{-dT}\leq1 give the displayed right side. Constants in (E21) may contain the fixed energy λ\lambda.

Here is the exact algebra allowing only first coefficient derivatives. In a Euclidean chart, for D=−i∂D=-i\partial, the difference ∫k(DαvDβv¯−DβvDαv¯)(E23) \int k\left(D^\alpha v\,\overline{D^\beta v} -D^\beta v\,\overline{D^\alpha v}\right) \tag{E23} is a finite sum with multiplier DlkD_lk, total derivative order |α|+|β|−1|\alpha|+|\beta|-1, and each individual order no greater than max⁡(|α|,|β|)\max(|\alpha|,|\beta|). This is the derivative-exchange result in Section 4 of Curved weights and the directions in which support can end. It follows by transferring an unmatched derivative once; when the two factors have equal orders, interchange one derivative from each factor before continuing. Each transfer differentiates kk once in its own integral. One never differentiates that error again.

For a sphere chart with smooth density ρdy\rho\,dy, replace kk by ρk\rho k. Its derivative is ρDlk+kDlρ\rho D_lk+kD_l\rho, so the estimate contains both |dk||dk| and |k||k|, with bounded chart constants. Expanding a word of sphere fields into coordinate derivatives produces its leading coordinate monomials and lower-order terms with bounded smooth coefficients. Reordering two sphere fields costs their commutator, a smooth first-order field. These costs also lower the total derivative count by one. The finite atlas has uniform bounds on these smooth factors.

For later use, attach degree one both to τ\tau and to each derivative. A differential polynomial of degree at most two and its formal complex conjugate have equal squared principal symbols. Expanding their squared norms, pairing terms with indices (α,β)(\alpha,\beta) and (β,α)(\beta,\alpha), and using (E23) therefore removes every term of total degree four without differentiating a coefficient twice. The remaining terms have the form (E19). If one factor was multiplication by Λ\Lambda, the degree-two exchange leaves at most one derivative on VV, or one power of τ\tau and no derivative, and (E21) gives exactly (E22). Terms of degree below two already satisfy the same counts. This proves the assertion for every pair of monomials; linearity and the finite number of monomials prove it for their sums.

In this argument “formal complex conjugate” is an algebraic operation on the displayed polynomial, not the assertion that the resulting operator is the Hilbert adjoint. We never expand the actual adjoint of a rough second-order monomial: doing so could introduce distributional second derivatives of its coefficient. Instead each paired integral exchange differentiates its combined multiplier once. Reversing the order of smooth sphere fields and using their divergence corrections costs only the lower-degree geometric terms described above. This distinction is essential for Lipschitz coefficients.

4. A Fourier inequality across a characteristic shell

Let y=(y′,yn)∈ℝny=(y',y_n)\in\mathbb R^n, A,τ≥1A,\tau\geq1, K>0K>0, M≥0M\geq0, and Lτ=Δy′+(∂yn−τ)2. L_\tau=\Delta_{y'}+(\partial_{y_n}-\tau)^2. Assume the four conditions A−ητ2≤τ3/K+A2,τ3/K≤A−ητ2+A2,M2K≤τA2,M≤A1−η/2.(E24) \begin{gathered} A^{-\eta}\tau^2\leq\tau^3/K+A^2, \qquad \tau^3/K\leq A^{-\eta}\tau^2+A^2,\\ M^2K\leq\tau A^2, \qquad M\leq A^{1-\eta/2}. \end{gathered} \tag{E24} Then, for v∈Cc∞(ℝn)v\in C_c^\infty(\mathbb R^n), K−1∑|α|≤2τ4−2|α|∥Dαv∥2+A−ητ3∥v∥2+M∑|α|≤1τ2−2|α|∥Dαv∥2≤C(K−1∥Lτv∥2+τA−η∑j<n∥Djv∥2+τA2∥v∥2).(E25) \begin{split} &K^{-1}\sum_{|\alpha|\leq2}\tau^{4-2|\alpha|}\|D^\alpha v\|^2 +A^{-\eta}\tau^3\|v\|^2 +M\sum_{|\alpha|\leq1}\tau^{2-2|\alpha|}\|D^\alpha v\|^2\\ &\quad\leq C\left(K^{-1}\|L_\tau v\|^2 +\tau A^{-\eta}\sum_{j<n}\|D_jv\|^2 +\tau A^2\|v\|^2\right). \end{split} \tag{E25} The constant depends only on dimension. The same proof works in dimension one, with the angular sum empty.

Proof. Put S=|ξ|2+τ2S=|\xi|^2+\tau^2 and q(ξ)=|ξ|2−τ2+2iτξn. q(\xi)=|\xi|^2-\tau^2+2i\tau\xi_n. The Fourier symbol of LτL_\tau is −q-q, so its modulus is |q||q|. The finite monomial sums on the left of (E25) are comparable, with dimensional constants, to K−1S2+A−ητ3+MS.(E26) K^{-1}S^2+A^{-\eta}\tau^3+MS. \tag{E26} It suffices to bound this by C(K−1|q|2+τA−η|ξ′|2+τA2)C(K^{-1}|q|^2+\tau A^{-\eta}|\xi'|^2+\tau A^2).

First suppose ||ξ′/τ|2−1|≥12or|ξn/τ|≥12.(E27) \left||\xi'/\tau|^2-1\right|\geq\tfrac12 \quad\text{or}\quad |\xi_n/\tau|\geq\tfrac12. \tag{E27} On this set S≤C|q|S\leq C|q|. For completeness, divide by τ2\tau^2 and put z=ξ/τz=\xi/\tau. For |z|≥2|z|\geq2, the real part |z|2−1|z|^2-1 bounds a fixed multiple of 1+|z|21+|z|^2. On |z|≤2|z|\leq2, the closed subset (E27) is compact and contains no zero of |z|2−1+2izn|z|^2-1+2iz_n: such a zero has zn=0z_n=0 and |z′|=1|z'|=1, excluded by (E27). Its modulus therefore has a positive minimum. These two regions prove the claimed uniform bound. The first condition in (E24), multiplied by τ\tau, controls A−ητ3A^{-\eta}\tau^3 by τ4/K+τA2\tau^4/K+\tau A^2. Since S≥τ2S\geq\tau^2, its first term is bounded by CS2/KCS^2/K, and hence by C|q|2/KC|q|^2/K. Finally MS≤12K−1S2+12M2K≤12K−1S2+12τA2.(E28) MS\leq\tfrac12K^{-1}S^2+\tfrac12M^2K \leq\tfrac12K^{-1}S^2+\tfrac12\tau A^2. \tag{E28} This proves the bound away from the shell.

On the complementary set, |ξ′|2≥τ2/2|\xi'|^2\geq\tau^2/2, |ξ′|2≤3τ2/2|\xi'|^2\leq3\tau^2/2, and |ξn|≤τ/2|\xi_n|\leq\tau/2. Thus S≍τ2S\asymp\tau^2. The second condition in (E24), multiplied by τ\tau, controls τ4/K\tau^4/K by τ3A−η+τA2\tau^3A^{-\eta}+\tau A^2. The angular term already controls A−ητ3A^{-\eta}\tau^3. The last condition gives Mτ2≤A1−η/2τ2=(τ3A−η)(τA2)≤12τ3A−η+12τA2.(E29) M\tau^2\leq A^{1-\eta/2}\tau^2 =\sqrt{(\tau^3A^{-\eta})(\tau A^2)} \leq\tfrac12\tau^3A^{-\eta}+\tfrac12\tau A^2. \tag{E29} Every term in (E26) is now bounded. The two sets may share their boundaries; the constants are uniform there. Multiply the pointwise inequality by |v̂|2|\widehat v|^2, integrate, and apply Plancherel. Its fixed normalization factor cancels from both sides. This proves (E25). ▫\square

5. Choosing the radius-dependent coefficient

The potential in (E11) is of size A2A^2 on a slab where eT≍Ae^T\asymp A. To place its square in the τA2∥V∥2\tau A^2\|V\|^2 term of (E25), we also require A2/K≤τ.(E30) A^2/K\leq\tau. \tag{E30} An admissible choice, of the smallest order allowed by the lower bounds, is K={Aητ,A2+η≤τ2,τ3/A2,A2≤τ2≤A2+η,A2/τ,τ2≤A2.(E31) K= \begin{cases} A^\eta\tau,& A^{2+\eta}\leq\tau^2,\\ \tau^3/A^2,& A^2\leq\tau^2\leq A^{2+\eta},\\ A^2/\tau,& \tau^2\leq A^2. \end{cases} \tag{E31} Both formulas agree at each transition. This is an optimization up to absolute constants, not a claim of an exact unique minimizer.

Here are all the checks. In the first region τ3/K=A−ητ2\tau^3/K=A^{-\eta}\tau^2, so the first two conditions in (E24) hold, and (E30) follows from A2−η≤τ2A^{2-\eta}\leq\tau^2. In the middle region τ3/K=A2\tau^3/K=A^2, while A−ητ2≤A2A^{-\eta}\tau^2\leq A^2; the first two conditions again hold. Moreover A2/K=A4/τ3≤τA^2/K=A^4/\tau^3\leq\tau since A2≤τ2A^2\leq\tau^2. In the last region A2/K=τA^2/K=\tau and τ3/K=τ4/A2≤A2\tau^3/K=\tau^4/A^2\leq A^2; also A−ητ2≤A2A^{-\eta}\tau^2\leq A^2, proving both conditions.

In these three regions, respectively, τA2K=A2−η,A4/τ2≥A2−η,τ2.(E32) \frac{\tau A^2}{K} =A^{2-\eta},\quad A^4/\tau^2\geq A^{2-\eta}, \quad\tau^2. \tag{E32} Therefore the remaining two conditions in (E24) hold whenever M≤min⁡(A1−η/2,τ).(E33) M\leq\min(A^{1-\eta/2},\tau). \tag{E33} The inequality K≥AK\geq A also holds in every region. In the first, τ≥A1+η/2\tau\geq A^{1+\eta/2} and hence K≥A1+3η/2K\geq A^{1+3\eta/2}. In the middle, τ≥A\tau\geq A, giving τ3/A2≥A\tau^3/A^2\geq A. In the last, τ≤A\tau\leq A, giving A2/τ≥AA^2/\tau\geq A.

For the eventual estimate set M=(e−T0/2+τ−1)−1.(E34) M=\left(e^{-T_0/2}+\tau^{-1}\right)^{-1}. \tag{E34} This has M≤τM\leq\tau and M≤eT0/2M\leq e^{T_0/2}. On a slab |T−log⁡A|<1|T-\log A|<1 meeting T>T0T>T_0, one has A>eT0−1A>e^{T_0-1}. Since η<1\eta<1, increasing the fixed threshold for T0T_0 ensures eT0/2≤e(1−η/2)(T0−1)≤A1−η/2. e^{T_0/2}\leq e^{(1-\eta/2)(T_0-1)}\leq A^{1-\eta/2}. Thus (E33) holds uniformly for every slab. Also M≥1M\geq1 when both T0T_0 and τ\tau are sufficiently large. There is no factor η\eta in the exponent −T0/2-T_0/2 in (E34).

To verify the asserted scale optimality, the second condition in (E24) and (E30) imply K≥max⁡(A2τ,τ3A−ητ2+A2).(E35) K\geq\max\left(\frac{A^2}{\tau}, \frac{\tau^3}{A^{-\eta}\tau^2+A^2}\right). \tag{E35} When A−ητ2≥A2A^{-\eta}\tau^2\geq A^2, the second term is between Aητ/2A^\eta\tau/2 and AητA^\eta\tau, and dominates the first up to constants. When A−ητ2≤A2A^{-\eta}\tau^2\leq A^2, it is between τ3/(2A2)\tau^3/(2A^2) and τ3/A2\tau^3/A^2; comparison with A2/τA^2/\tau divides this range at τ2=A2\tau^2=A^2. This proves that (E31) is within a factor two of the necessary lower bound.

6. Derivative recovery in one chart and one slab

Rotate the sphere to center a chart at its north pole and use y=(ω1,…,ωn−1)y=(\omega_1,\ldots,\omega_{n-1}) with |y|<r<1|y|<r<1. The last coordinate is 1−|y|2\sqrt{1-|y|^2}. The induced metric and its inverse give dω=(1−|y|2)−1/2dy,ΔS=∑i,j<n(δij−yiyj)∂i∂j−(n−1)∑i<nyi∂i,∑j|Ωjv|2=∑i,j<n(δij−yiyj)∂iv∂jv¯.(E36) \begin{split} d\omega&=(1-|y|^2)^{-1/2}\,dy,\\ \Delta_S&=\sum_{i,j<n}(\delta_{ij}-y_iy_j)\partial_i\partial_j -(n-1)\sum_{i<n}y_i\partial_i,\\ \sum_j|\Omega_jv|^2 &=\sum_{i,j<n}(\delta_{ij}-y_iy_j) \partial_iv\,\overline{\partial_jv}. \end{split} \tag{E36} For example, the density is the square root of the determinant of I+yyt/(1−|y|2)I+yy^t/(1-|y|^2), and the inverse matrix is I−yytI-yy^t. Substituting these into the divergence formula for the Laplace–Beltrami operator gives the middle identity. Thus the coordinate gradient norm and the angular gradient norm are comparable with fixed constants on a fixed small chart. The same is true through order two after adding lower orders, by expanding each field and expressing each coordinate derivative in the spanning fields.

Suppose VV is supported in this chart and in |T−log⁡A|<1|T-\log A|<1, T>T0T>T_0. In these coordinates write Qτ=Lτ+E2+E1+Λ(T),Lτ=Δy+(∂T−τ)2.(E37) Q_\tau=L_\tau+E_2+E_1+\Lambda(T), \quad L_\tau=\Delta_y+(\partial_T-\tau)^2. \tag{E37} The polynomial E2E_2 has total degree at most two in derivatives and τ\tau, with coefficients bounded by C(r+e−ηT0)C(r+e^{-\eta T_0}). It includes the variable principal coefficients and all their conjugated τ\tau-terms. The polynomial E1E_1 has total degree at most one, with uniformly bounded coefficients; it includes c(∂T−τ)c(\partial_T-\tau) and the bounded first-order sphere terms. To see these bounds directly, subtract the leading constant matrix in (E36), use a−1=O(e−ηT)a-1=O(e^{-\eta T}), and use (E12). No derivative of a rough coefficient is used in this step.

Put HK(V)=K−1∑|α|≤2τ4−2|α|∥DαV∥2 H_K(V)=K^{-1}\sum_{|\alpha|\leq2} \tau^{4-2|\alpha|}\|D^\alpha V\|^2 in the coordinate chart. Expanding the finite polynomials in (E37) gives K−1∥E2V∥2≤C(r+e−ηT0)2HK(V),K−1∥E1V∥2≤Cτ−2HK(V).(E38) K^{-1}\|E_2V\|^2\leq C(r+e^{-\eta T_0})^2H_K(V),\qquad K^{-1}\|E_1V\|^2\leq C\tau^{-2}H_K(V). \tag{E38} Use (E25) and LτV=QτV−E2V−E1V−ΛVL_\tau V=Q_\tau V-E_2V-E_1V-\Lambda V. Choose the fixed chart radius small first, then choose fixed sufficiently large lower thresholds for T0T_0 and τ\tau, so the contributions (E38) consume at most half of HKH_K. The equivalence of the smooth density norms changes only fixed constants. The potential contributes K−1∥ΛV∥2≤CA4K−1∥V∥2≤CτA2∥V∥2,(E39) K^{-1}\|\Lambda V\|^2\leq C A^4K^{-1}\|V\|^2 \leq C\tau A^2\|V\|^2, \tag{E39} where (E30) is used. This is a bound by the designated potential term on the right, with no smallness assertion about Λ\Lambda.

On the slab, powers of AA and eTe^T are comparable by constants determined by its fixed width. After (E38) has been absorbed, one may drop the factors τ4−2|α|≥1\tau^{4-2|\alpha|}\geq1 in the retained first sum. We obtain K−1∑k=02∥𝒟kV∥2+F(V)+M(τ2∥V∥2+∥𝒟1V∥2)≤C(K−1∥QτV∥2+τ∑j∥e−ηT/2ΩjV∥2+τ∥eTV∥2).(E40) \begin{split} &K^{-1}\sum_{k=0}^2\|\mathcal D^kV\|^2+F(V) +M\bigl(\tau^2\|V\|^2+\|\mathcal D^1V\|^2\bigr)\\ &\quad\leq C\left(K^{-1}\|Q_\tau V\|^2 +\tau\sum_j\|e^{-\eta T/2}\Omega_jV\|^2 +\tau\|e^TV\|^2\right). \end{split} \tag{E40} The first sum here deliberately has no remaining powers of τ\tau. Its stronger predecessor was needed for the coefficient absorption; (E40) alone would not justify that absorption.

Now use (E31) and (E34). The inequality K≥AK\geq A gives K−1≤A−1≍e−TK^{-1}\leq A^{-1}\asymp e^{-T}. The third condition in (E24) gives K−1≥M2τA2≥MτA2,(E41) K^{-1}\geq\frac{M^2}{\tau A^2} \geq\frac{M}{\tau A^2}, \tag{E41} where M≥1M\geq1 is used in the second step. Retain this lower bound only for order two in (E40), and keep the displayed MM-weighted lower orders. It follows that MW(V)+F(V)≤C(∥e−T/2QτV∥2+τ∑j∥e−ηT/2ΩjV∥2+τ∥eTV∥2).(E42) \begin{split} M W(V)+F(V)\leq C\bigg(&\|e^{-T/2}Q_\tau V\|^2 +\tau\sum_j\|e^{-\eta T/2}\Omega_jV\|^2 +\tau\|e^TV\|^2\bigg). \end{split} \tag{E42} This proves the required derivative estimate on each chart and slab, with constants independent of their location.

7. Localization with constants independent of support

We now prove (E42) for every V∈Cc∞((T0,∞)×Sn−1)V\in C_c^\infty((T_0,\infty)\times S^{n-1}). Choose finitely many real smooth functions ϕj\phi_j, supported in charts of the fixed size used above, with ∑jϕj2=1\sum_j\phi_j^2=1. Such a square partition is obtained from any nonnegative subordinate partition by dividing its members by the square root of the sum of their squares. The denominator is smooth and strictly positive on the compact sphere.

Choose a real nonnegative smooth function supported in (−1,1)(-1,1), positive on [−3/4,3/4][-3/4,3/4]. Normalize it by the square root of the sum of the squares of its integer translates. The result is a smooth ψ\psi, with supp⁡ψ⊂(−1,1)\operatorname{supp}\psi\subset(-1,1), such that ∑k∈ℤψ(T−k)2=1. \sum_{k\in\mathbb Z}\psi(T-k)^2=1. The denominator is smooth, periodic, and bounded away from zero. All derivatives of ψ(T−k)\psi(T-k) of any fixed order are bounded uniformly in kk. Put χjk(T,ω)=ϕj(ω)ψ(T−k),∑j,kχjk2=1.(E43) \chi_{jk}(T,\omega)=\phi_j(\omega)\psi(T-k),\qquad \sum_{j,k}\chi_{jk}^2=1. \tag{E43} Only a bounded number of these functions meet a point. A slab meeting supp⁡V\operatorname{supp}V has k>T0−1k>T_0-1, so (E34) is admissible with A=ekA=e^k, including slabs whose lower endpoint is below T0T_0. The function χjkV\chi_{jk}V itself still has compact support above T0T_0.

Apply (E42) to these functions and sum. Zeroth-order terms sum exactly. For each real field YY in 𝒟\mathcal D, expansion and ∑χjkYχjk=0\sum\chi_{jk}Y\chi_{jk}=0 give ∑j,k|Y(χjkV)|2=|YV|2+∑j,k|Yχjk|2|V|2.(E44) \sum_{j,k}|Y(\chi_{jk}V)|^2 =|YV|^2+\sum_{j,k}|Y\chi_{jk}|^2|V|^2. \tag{E44} For order two, the product rule shows that χjkY1Y2V\chi_{jk}Y_1Y_2V equals Y1Y2(χjkV)Y_1Y_2(\chi_{jk}V) minus terms bounded by C(|𝒟1V|+|V|)C(|\mathcal D^1V|+|V|) on the cutoff support. Squaring, summing, and using bounded overlap yields W(V)≤C∑j,kW(χjkV)+Cτ−1e−2T0(∥𝒟1V∥2+∥V∥2). W(V)\leq C\sum_{j,k}W(\chi_{jk}V) +C\tau^{-1}e^{-2T_0} (\|\mathcal D^1V\|^2+\|V\|^2). The last term is absorbed into W(V)W(V) after increasing the parameter thresholds. Thus the summed left sides control MW(V)+F(V)MW(V)+F(V), up to fixed constants.

The growing potential commutes with all cutoffs. In the other terms of QτQ_\tau, two derivatives may hit χ\chi, or one may hit χ\chi and one may remain on VV. Conjugation supplies at most one τ\tau in a nonzero commutator, since a τ2\tau^2 term is multiplication. Explicitly, [∂T2,χ]V=2χTVT+χTTV,[−2τ∂T,χ]V=−2τχTV, [\partial_T^2,\chi]V=2\chi_TV_T+\chi_{TT}V,\qquad [-2\tau\partial_T,\chi]V=-2\tau\chi_TV, and [Y1Y2,χ]V=(Y1Y2χ)V+(Y2χ)Y1V+(Y1χ)Y2V[Y_1Y_2,\chi]V=(Y_1Y_2\chi)V+(Y_2\chi)Y_1V+(Y_1\chi)Y_2V. Coefficients stay on the left and are uniformly bounded; none is differentiated. It follows that ∑j,k∥e−T/2[Qτ,χjk]V∥2≤Ce−T0(∥𝒟1V∥2+τ2∥V∥2)≤Ce−T0W(V).(E45) \sum_{j,k}\|e^{-T/2}[Q_\tau,\chi_{jk}]V\|^2 \leq C e^{-T_0} (\|\mathcal D^1V\|^2+\tau^2\|V\|^2) \leq C e^{-T_0}W(V). \tag{E45} The angular right-side terms in (E42) contribute, besides a fixed multiple of the original angular norm, at most Cτ∥e−ηT/2V∥2=Cτ−2F(V)C\tau\|e^{-\eta T/2}V\|^2=C\tau^{-2}F(V). The potential norm sums exactly. Therefore the only additional right-side errors are Ce−T0W+Cτ−2FCe^{-T_0}W+C\tau^{-2}F. They are absorbed by MW+FMW+F for large thresholds, since M≥1M\geq1. This proves the global estimate (E42). The number of slabs occupied by VV never enters its constant.

8. A norm identity revealing the two positive terms

For the moment set B=0B=0 in (E11). Define H=∂T2+a(T)ΔS+τ2−c(T)τ+Λ(T),J=−β(T)∂T,β(T)=2τ−c(T).(E46) \begin{split} H&=\partial_T^2+a(T)\Delta_S+\tau^2-c(T)\tau+\Lambda(T),\\ J&=-\beta(T)\partial_T,\qquad \beta(T)=2\tau-c(T). \end{split} \tag{E46} Then Q0,τ=H+JQ_{0,\tau}=H+J, and its algebraically reversed companion is Q0,τ−=H−JQ_{0,\tau}^-=H-J. With respect to dTdωdT\,d\omega, H*=HH^*=H and J*=−J−c′J^*=-J-c'. Hence ∥Q0,τV∥2−∥Q0,τ−V∥2=4Re⁡⟨HV,JV⟩=2Re⁡⟨[H,J]V,V⟩−2Re⁡⟨c′HV,V⟩.(E47) \|Q_{0,\tau}V\|^2-\|Q_{0,\tau}^-V\|^2 =4\operatorname{Re}\langle HV,JV\rangle =2\operatorname{Re}\langle[H,J]V,V\rangle -2\operatorname{Re}\langle c'HV,V\rangle. \tag{E47} The real part makes this identity independent of which slot of the complex inner product is chosen linear.

We compute it completely. Since β′=−c′\beta'=-c', [∂T2,−β∂T]=2c′∂T2+c″∂T,[aΔS,−β∂T]=βa′ΔS,[τ2−cτ+Λ,−β∂T]=β(−τc′+Λ′).(E48) \begin{split} [\partial_T^2,-\beta\partial_T]&=2c'\partial_T^2+c''\partial_T,\\ [a\Delta_S,-\beta\partial_T]&=\beta a'\Delta_S,\\ [\tau^2-c\tau+\Lambda,-\beta\partial_T] &=\beta(-\tau c'+\Lambda'). \end{split} \tag{E48} These derivatives concern the smooth scalar functions a,c,Λa,c,\Lambda, not a rough principal coefficient. Insert (E48) in (E47). Integration by parts in TT combines 2c′∂T2+2c″∂T2c'\partial_T^2+2c''\partial_T into −2c′|VT|2-2c'|V_T|^2; the angular integration uses (E7). Thus the exact identity is ∥Q0,τV∥2−∥Q0,τ−V∥2=∫[−2c′|VT|2−2(βa′−c′a)∑j|ΩjV|2+((−6τ2+4cτ)c′+2βΛ′−2c′Λ)|V|2]dTdω.(E49) \begin{split} &\|Q_{0,\tau}V\|^2-\|Q_{0,\tau}^-V\|^2\\ &=\int\bigg[ -2c'|V_T|^2 -2(\beta a'-c'a)\sum_j|\Omega_jV|^2\\ &\hspace{25mm} +\Big((-6\tau^2+4c\tau)c' +2\beta\Lambda'-2c'\Lambda\Big)|V|^2 \bigg]\,dT\,d\omega. \end{split} \tag{E49} This identity is also a useful sign check on the direction of the curved radial adjustment.

Let s=e−ηTs=e^{-\eta T}. We have a′=−2η2sha'=-2\eta^2s h, c=O(1)c=O(1), and c′=O(s)c'=O(s). Therefore −2(βa′−c′a)=4(2τ−c)η2sh+2c′a≥4η2τs(E50) -2(\beta a'-c'a)=4(2\tau-c)\eta^2s h+2c'a \geq4\eta^2\tau s \tag{E50} for sufficiently large τ\tau, uniformly for large TT. The first term in (E49) is bounded below by −C∥VT∥2-C\|V_T\|^2. The part (−6τ2+4cτ)c′(-6\tau^2+4c\tau)c' is bounded below by −Cτ2|V|2-C\tau^2|V|^2, so both of these costs lie in CR(V)CR(V). By (E13), and by enlarging T0,τT_0,\tau if needed, 2βΛ′−2c′Λ≥32λτe2T.(E51) 2\beta\Lambda'-2c'\Lambda \geq\tfrac32\lambda\tau e^{2T}. \tag{E51} For example β≥3τ/2\beta\geq3\tau/2 for large τ\tau, while |c′Λ|≤Cλse2T|c'\Lambda|\leq C\lambda s e^{2T}, which is absorbed in the excess above 3λτe2T/23\lambda\tau e^{2T}/2. Combining (E49)–(E51) gives ∥Q0,τ−V∥2+4η2τ∑j∥e−ηT/2ΩjV∥2+32λτ∥eTV∥2≤∥Q0,τV∥2+CR(V).(E52) \|Q_{0,\tau}^-V\|^2 +4\eta^2\tau\sum_j\|e^{-\eta T/2}\Omega_jV\|^2 +\tfrac32\lambda\tau\|e^TV\|^2 \leq\|Q_{0,\tau}V\|^2+CR(V). \tag{E52} The reserve λτ∥eTV∥2/2\lambda\tau\|e^TV\|^2/2 will pay for the coefficient-potential products.

9. Restoring complex Lipschitz coefficients

Let BτB_\tau be the conjugate of BB in (E11). Define Bτ−=∑j+|α|≤2bαj¯(−∂T−τ)j(−Ω)α,Qτ−=Q0,τ−+Bτ−.(E53) B_\tau^-= \sum_{j+|\alpha|\leq2}\overline{b_{\alpha j}}\, (-\partial_T-\tau)^j(-\Omega)^\alpha, \qquad Q_\tau^-=Q_{0,\tau}^-+B_\tau^-. \tag{E53} The order of each displayed word is preserved. This reversal is well defined for locally Lipschitz coefficients because it does not differentiate them. It is not identified with Qτ*Q_\tau^*.

Subtract the background difference (E47) from ∥QτV∥2−∥Qτ−V∥2\|Q_\tau V\|^2-\|Q_\tau^-V\|^2. We examine every type of resulting product.

Products with the potential. The terms are 2Re⁡(⟨BτV,ΛV⟩−⟨Bτ−V,ΛV⟩). 2\operatorname{Re} \left(\langle B_\tau V,\Lambda V\rangle -\langle B_\tau^-V,\Lambda V\rangle\right). For a second-order monomial the terms without a derivative on its coefficient cancel after one exchange of derivatives. The remaining integrals have one derivative on Λbαj\Lambda b_{\alpha j} and at most one derivative on VV. A first-order monomial leaves a zeroth-order product; its conjugation can contribute one τ\tau. For a zeroth-order monomial the real parts cancel without integration, including the term with two powers of τ\tau produced by conjugating a radial second derivative. Indeed Re⁡(Λbτ2|V|2)=Re⁡(Λb‾τ2|V|2)\operatorname{Re}(\Lambda b\tau^2|V|^2)=\operatorname{Re}(\Lambda\bar b\tau^2|V|^2) since Λ\Lambda is real. Thus no term τ2e(1−d)T|V|2\tau^2e^{(1-d)T}|V|^2 remains in this class. The same statements follow for angular words by the density and adjoint calculation in Section 3. Thus the total absolute value is bounded by C∫e(1−d)T(τ|V|2+|𝒟1V||V|)≤∥eTV∥2+C(τ2∥V∥2+∥𝒟1V∥2).(E54) C\int e^{(1-d)T} \left(\tau|V|^2+|\mathcal D^1V|\,|V|\right) \leq \|e^TV\|^2 +C\bigl(\tau^2\|V\|^2+\|\mathcal D^1V\|^2\bigr). \tag{E54} Here (E21)–(E22) were used. For sufficiently large τ\tau, the first term is at most the potential reserve in (E52), while the rest lies in CRCR.

Products with one perturbation coefficient and no potential. Expand the powers (∂T−τ)j(\partial_T-\tau)^j in BτB_\tau, and the corresponding reversed powers in Bτ−B_\tau^-. Each term has degree at most two. All products of total degree four cancel at principal-symbol level by the exchange identity (E23). Terms left by that exchange have degree at most three, individual derivative orders at most two, and a multiplier bounded by Ce−(1+d)TCe^{-(1+d)T}. The multiplier is a product of one perturbation coefficient with smooth background factors or its first derivative; all such quantities satisfy this bound by (E12). Commutators of sphere fields and their divergence corrections also have this bound and lower the differential order by one. Every resulting integral is therefore one of the finitely many types (E19), and is bounded by CRCR by (E20) and its lower-order case.

One can check the cancellation directly in coordinate DD-notation. Write the leading polynomial as ∑τjkαjDα\sum \tau^j k_{\alpha j}D^\alpha. Its reversed partner has the conjugate leading coefficients. In the difference of the two squared norms, swap the two coefficient indices in the second sum. The coefficient of the derivative product is then the same in both sums, leaving exactly the antisymmetric combination (E23). Each application of (E23) consumes one derivative, leaving j+|μ|+|ν|≤3j+|\mu|+|\nu|\leq3. Lower-degree pieces that arise when an ordered field word is expanded already have this loss. This also shows why the individual order may remain two.

Products with two perturbation coefficients. Apply the same paired expansion to ∥BτV∥2−∥Bτ−V∥2\|B_\tau V\|^2-\|B_\tau^-V\|^2. A multiplier is now a product of two perturbation coefficients; it and its first derivatives are O(e−2(1+d)T)O(e^{-2(1+d)T}). For T≥0T\geq0 this is bounded by Ce−(1+d)TCe^{-(1+d)T}. The same exchange removes the total-degree-four terms, and all remaining products again satisfy (E19). Their contribution is bounded by CRCR.

The three classes exhaust the squared-norm expansion. At no point is a differentiated coefficient differentiated again: the exchange identity is applied to each original multiplier, and its error integral is bounded immediately. Combining these bounds with (E52) proves ∥Qτ−V∥2+4η2τ∑j∥e−ηT/2ΩjV∥2+λτ∥eTV∥2≤∥QτV∥2+CR(V).(E55) \|Q_\tau^-V\|^2 +4\eta^2\tau\sum_j\|e^{-\eta T/2}\Omega_jV\|^2 +\lambda\tau\|e^TV\|^2 \leq\|Q_\tau V\|^2+CR(V). \tag{E55} The initial calculation uses smooth VV and Lipschitz coefficients. Weak integration by parts justifies the coefficient exchanges directly. Equivalently, one can first smooth the coefficients on a compact neighborhood, use their uniform Lipschitz bounds in the finite formulas, and pass to the limit without introducing any second-derivative coefficient bound.

10. Recovering the longitudinal energy

The radial derivative does not occur with a useful sign in (E55), so we recover it from the difference of the operators. Equations (E46) and (E53) give 12(Qτ−Qτ−)V=−(2τ−c)VT+12(Bτ−Bτ−)V.(E56) \frac12(Q_\tau-Q_\tau^-)V =-(2\tau-c)V_T+\frac12(B_\tau-B_\tau^-)V. \tag{E56} By direct expansion of these finite polynomials, |(Bτ−Bτ−)V|≤Ce−(1+d)T∑k=02τ2−k|𝒟kV|.(E57) |(B_\tau-B_\tau^-)V| \leq C e^{-(1+d)T} \sum_{k=0}^2\tau^{2-k}|\mathcal D^kV|. \tag{E57} Since 2τ−c≍τ2\tau-c\asymp\tau uniformly, the triangle inequality and the square of a finite sum imply τ2∥VT∥2≤C(∥QτV∥2+∥Qτ−V∥2+∑k=02τ4−2k∥e−(1+d)T𝒟kV∥2).(E58) \tau^2\|V_T\|^2\leq C\left( \|Q_\tau V\|^2+\|Q_\tau^-V\|^2 +\sum_{k=0}^2\tau^{4-2k} \|e^{-(1+d)T}\mathcal D^kV\|^2\right). \tag{E58} Divide by τ\tau. For k=2k=2, the error is at most τ−1∥e−T𝒟2V∥2\tau^{-1}\|e^{-T}\mathcal D^2V\|^2. For k=0,1k=0,1, it is at most the corresponding decaying term τ3−2k∥e−dT𝒟kV∥2\tau^{3-2k}\|e^{-dT}\mathcal D^kV\|^2. Thus the divided error is bounded by CRCR. Equation (E55) also gives ∥Qτ−V∥2≤∥QτV∥2+CR\|Q_\tau^-V\|^2\leq\|Q_\tau V\|^2+CR. Insert this in the divided version of (E58), and add the positive terms from (E55), decreasing their fixed coefficients if necessary. We obtain X(V):=η2τ∑j∥e−ηT/2ΩjV∥2+τ∥VT∥2+λτ∥eTV∥2≤CE(∥QτV∥2+R(V)).(E59) X(V):=\eta^2\tau\sum_j\|e^{-\eta T/2}\Omega_jV\|^2 +\tau\|V_T\|^2+\lambda\tau\|e^TV\|^2 \leq C_E\bigl(\|Q_\tau V\|^2+R(V)\bigr). \tag{E59} The division by τ\tau in this argument is what puts the second-derivative perturbation into the exact remainder (E18).

11. Closing the two estimates in a fixed order

Put P=∥QτV∥2P=\|Q_\tau V\|^2, and retain the entire XX from (E59), including the radial term. The global form of (E42) says MW+F≤CS(e−T0P+a0X),(E60) MW+F\leq C_S(e^{-T_0}P+a_0X), \tag{E60} where a0a_0 is a fixed constant large enough to include η−2\eta^{-2} and λ−1\lambda^{-1}.

Let s0=e(η−2d)T0s_0=e^{(\eta-2d)T_0}. Since η<d\eta<d, it tends to zero as T0→∞T_0\to\infty. For T≥T0T\geq T_0, e−2dT≤s0e−ηTe^{-2dT}\leq s_0e^{-\eta T}. The zeroth-order decaying part of RR is therefore at most s0Fs_0F. Its first-order angular part is bounded by Cs0η−2XC s_0\eta^{-2}X. The radial part obeys τ∥e−dTVT∥2≤s0τ∥e−ηT/2VT∥2≤s0τ∥VT∥2≤s0X. \tau\|e^{-dT}V_T\|^2 \leq s_0\tau\|e^{-\eta T/2}V_T\|^2 \leq s_0\tau\|V_T\|^2\leq s_0X. Consequently R≤W+C0s0(F+a0X).(E61) R\leq W+C_0s_0(F+a_0X). \tag{E61} This is the step at which discarding the radial term in (E59) would leave an error uncontrolled.

From (E60), both W≤CSM−1(e−T0P+a0X)W\leq C_SM^{-1}(e^{-T_0}P+a_0X) and F≤CS(e−T0P+a0X)F\leq C_S(e^{-T_0}P+a_0X). Substitution into (E61) yields R≤CS(M−1+C0s0)e−T0P+a0[CS(M−1+C0s0)+C0s0]X.(E62) \begin{split} R\leq& C_S(M^{-1}+C_0s_0)e^{-T_0}P\\ &+a_0\left[C_S(M^{-1}+C_0s_0)+C_0s_0\right]X. \end{split} \tag{E62} Choose T0T_0 sufficiently large, then a sufficiently large lower threshold for τ\tau. Because M−1=e−T0/2+τ−1M^{-1}=e^{-T_0/2}+\tau^{-1}, these choices make the coefficient of XX in CEC_E times (E62) at most 1/21/2, and the coefficient of PP at most one. All earlier thresholds can be included by taking their maximum. Equation (E59) then gives X≤2(CE+1)P.(E63) X\leq2(C_E+1)P. \tag{E63} Substitute (E63) back into (E60): W≤CM−1PW\leq CM^{-1}P. The potential term in XX gives ∥eTV∥2≤Cτ−1P≤CM−1P\|e^TV\|^2\leq C\tau^{-1}P\leq CM^{-1}P. Together these prove (E17). The constants work for every T0T_0 and τ\tau above the chosen fixed thresholds.

Finally, undo the conjugation. Angular fields commute with eτTe^{\tau T}, and eτTUT=VT−τV. e^{\tau T}U_T=V_T-\tau V. Thus (E17) implies ∥e(τ+1)TU∥2+∥eτTUT∥2+∑j∥eτTΩjU∥2≤C(e−T0/2+τ−1)∥eτTQU∥2.(E64) \|e^{(\tau+1)T}U\|^2 +\|e^{\tau T}U_T\|^2 +\sum_j\|e^{\tau T}\Omega_jU\|^2 \leq C\left(e^{-T_0/2}+\tau^{-1}\right) \|e^{\tau T}QU\|^2. \tag{E64} In fact the two displayed left sides are equal. For compactly supported VV, integration of ∂T|V|2\partial_T|V|^2 gives ∥VT−τV∥2=∥VT∥2+τ2∥V∥2, \|V_T-\tau V\|^2=\|V_T\|^2+\tau^2\|V\|^2, because the real part of ∫VTV¯\int V_T\overline V is zero. Together with the unchanged angular and potential norms, this proves the equivalence of (E17) and (E64); using (τ+eT)2(\tau+e^T)^2 in place of τ2+e2T\tau^2+e^{2T} only changes fixed constants. The estimate (E64) extends to compactly supported H2H^2 functions inside the cylinder. Approximate in H2H^2 on a fixed compact neighborhood of the support; the weights and coefficients are bounded there, and Q:H2→L2Q:H^2\to L^2 is continuous. The approximation is taken with τ\tau fixed. No parameter-uniform smoothing assertion is required.

The estimate for the full original operator and measure

Retain the original data of (E3a)–(E3f). For an original point xx, put rM(x)=|M−1x|r_M(x)=|M^{-1}x|, ωM(x)=M−1x/rM(x)\omega_M(x)=M^{-1}x/r_M(x), and let TM(x)T_M(x) be the unique solution of log⁡rM=TM−e−ηTM\log r_M=T_M-e^{-\eta T_M}. Its existence and smoothness for rM>0r_M>0 follow because the derivative h=1+ηe−ηTh=1+\eta e^{-\eta T} is strictly positive and the function ranges from −∞-\infty to +∞+\infty. The actual fields in the original coordinates are ℛ0=h(TM)∑lxl∂xl,ℛj=rM∑lMlj∂xl−(ωM)j∑lxl∂xl.(E77) \mathcal R_0=h(T_M)\sum_lx_l\partial_{x_l},\qquad \mathcal R_j=r_M\sum_lM_{lj}\partial_{x_l} -(\omega_M)_j\sum_lx_l\partial_{x_l}. \tag{E77} For W(T,ω)=w(et(T)Mω)W(T,\omega)=w(e^{t(T)}M\omega), the full chain rule gives ∂TW=(ℛ0w)(x)\partial_TW=(\mathcal R_0w)(x) and ΩjW=(ℛjw)(x)\Omega_jW=(\mathcal R_jw)(x). Repeated application preserves every ordered word, including all derivatives of a field coefficient. The exact operator and measure identities are QW=−σh(TM)2rM2((p−λ)w)(x),dx=|det⁡M|h(T)ent(T)dTdω.(E78) QW=-\sigma h(T_M)^2r_M^2((p-\lambda)w)(x),\qquad dx=|\det M|h(T)e^{nt(T)}\,dT\,d\omega. \tag{E78} Indeed (E8) applied to the complete auxiliary matrix, with its energy σλ\sigma\lambda, is multiplied by h2h^2, which proves the first identity. The second retains both the original constant linear Jacobian and the radial Jacobian, followed by dt=hdTdt=h\,dT.

Set r0=exp⁡(T0−e−ηT0)r_0=\exp(T_0-e^{-\eta T_0}), large enough that rM>r0r_M>r_0 lies in XX. Substituting both identities of (E78) into the proved estimate (E64), without deleting any measure or radial factor, gives for every original test function supported in this exterior region ∫rM>r0e2(τ+1)TM|w|2+e2τTM(|ℛ0w|2+∑j|ℛjw|2)|det⁡M|h(TM)rMndx≤C(e−T0/2+τ−1)∫rM>r0|σ(p−λ)w|2h(TM)4rM4e2τTM|det⁡M|h(TM)rMndx.(E79) \begin{split} &\int_{r_M>r_0} \frac{e^{2(\tau+1)T_M}|w|^2 +e^{2\tau T_M}\bigl(|\mathcal R_0w|^2+ \sum_j|\mathcal R_jw|^2\bigr)} {|\det M|h(T_M)r_M^n}\,dx\\ &\quad\leq C\bigl(e^{-T_0/2}+\tau^{-1}\bigr) \int_{r_M>r_0}|\sigma(p-\lambda)w|^2 \frac{h(T_M)^4r_M^4e^{2\tau T_M}} {|\det M|h(T_M)r_M^n}\,dx. \end{split} \tag{E79} The constants are those already proved for the full auxiliary coefficient error, sign and positive energy. The original operator, energy, solution coordinates and measure are explicit on both sides.

To verify that every Cartesian derivative has a receiving map, put 𝒱j=(ωM)jh(TM)−1ℛ0+ℛj\mathcal V_j=(\omega_M)_jh(T_M)^{-1}\mathcal R_0+\mathcal R_j. Then ∂xl=rM−1∑j(M−1)jl𝒱j,∂xl∂xq=rM−1∑j(M−1)jl𝒱j(rM−1∑k(M−1)kq𝒱k).(E80) \partial_{x_l}=r_M^{-1}\sum_j(M^{-1})_{jl}\mathcal V_j,\qquad \partial_{x_l}\partial_{x_q} =r_M^{-1}\sum_j(M^{-1})_{jl}\mathcal V_j \left(r_M^{-1}\sum_k(M^{-1})_{kq}\mathcal V_k\right). \tag{E80} The left field in the second identity acts on the whole bracket: it differentiates rM−1r_M^{-1}, ωM\omega_M, h−1h^{-1}, and the original function wherever the product rule requires. This follows from (E7) and the full matrix chain rule (E3c). Conversely, (E77) gives every field in terms of original Cartesian derivatives. Iteration through order two supplies both complete finite derivative arrays, with their original radial and matrix factors. The all-weight correspondence (E3f) therefore transfers the weak solution, annular regularity and every cutoff limit of Section 12 in both directions. Its exterior zero region is the actual ellipsoidal region |M−1x|>r0|M^{-1}x|>r_0, and the original domain and local inequality then receive the proved continuation argument.

The full original exterior coordinates, matrix and measure

For the displayed example, A∞=(4202)A_\infty=\left(\begin{smallmatrix}4&2\\0&2\end{smallmatrix}\right), σ=1\sigma=1, and det⁡M=7\det M=\sqrt7. The full auxiliary matrix is I+K∞I+K_\infty, with off-diagonal skew entries 1/71/\sqrt7 and −1/7-1/\sqrt7. The contours are the original coordinate surfaces |M−1x|=1,2|M^{-1}x|=1,2, rather than frequency surfaces. Equations (E3b)–(E3f) and (E77)–(E80) prove every map and factor in the diagram.

12. From weak decay to an actual open zero set

We prove the theorem of Section 1, beginning with the regularity needed to use (E64).

On every compact subset of X\{0}X\setminus\{0\}, (E5) and u∈Hloc1u\in H^1_{\mathrm{loc}} give pu∈L2pu\in L^2. Weak elliptic regularity in Sections 7–8 of Local inverses and distance-weighted elliptic estimates therefore gives u∈Hloc2(X\{0})u\in H^2_{\mathrm{loc}}(X\setminus\{0\}). The initially weak product is aDjv=Dj(av)−(Dja)v,v∈Lloc2. aD_jv=D_j(av)-(D_ja)v,\qquad v\in L^2_{\mathrm{loc}}. It agrees with the usual nondivergence expression after this regularity improvement. In particular no second derivatives were assumed in (E4).

We need this improvement with weights at infinity. Let AR={R<|x|<2R}A_R=\{R<|x|<2R\} and AR′={R/2<|x|<4R}A_R'=\{R/2<|x|<4R\}. For sufficiently large RR, both lie in XX. Scale x=Ryx=Ry and write uR(y)=u(Ry)u_R(y)=u(Ry). The coefficients a(Ry)a(Ry) on the fixed annulus {1/2<|y|<4}\{1/2<|y|<4\} have uniform ellipticity and a common modulus of continuity. Indeed they approach the identity uniformly, and their first yy-derivatives are bounded by CR−1−dCR^{-1-d}. The interior estimate in Section 6 of Local inverses and distance-weighted elliptic estimates, on a fixed pair of nested annuli, has a constant independent of RR. Scaling its m=p=2m=p=2 version back yields ∑k=02Rk∥Dku∥L2(AR)≤C(R2∥pu∥L2(AR′)+∥u∥L2(AR′)).(E65) \sum_{k=0}^2R^k\|D^ku\|_{L^2(A_R)} \leq C\left(R^2\|pu\|_{L^2(A_R')} +\|u\|_{L^2(A_R')}\right). \tag{E65} The same statement with a harmless separate first-order term on the right would also suffice; it follows from the stated estimate by the interior interpolation inequality. The factor R−n/2R^{-n/2} from scaling the L2L^2 norm occurs on both sides and cancels.

By (E5), R2∥pu∥L2(AR′)≤C((R2+R)∥u∥L2(AR′)+R∥Du∥L2(AR′)).(E66) R^2\|pu\|_{L^2(A_R')} \leq C\left((R^2+R)\|u\|_{L^2(A_R')} +R\|Du\|_{L^2(A_R')}\right). \tag{E66} For every N>0N>0, (E4) bounds the right side of (E66), and hence every term on the left of (E65), by CNR−NC_NR^{-N}. To see this directly, on AR′A_R' the function (1+|x|)s(1+|x|)^s is comparable to RsR^s; take s>N+2s>N+2 in (E4). It follows by summing dyadic annuli, whose enlarged annuli have bounded overlap, that (1+|x|)sDαu∈L2({|x|>R1})(s∈ℝ,|α|≤2).(E67) (1+|x|)^sD^\alpha u\in L^2(\{|x|>R_1\}) \quad(s\in\mathbb R,\ |\alpha|\leq2). \tag{E67} For a given ss, choose the annular exponent NN larger than s+1s+1; the squared annular estimates then sum as a convergent geometric series.

Every cylindrical derivative through order two is a bounded sum of ektDku(etω)e^{kt}D^ku(e^t\omega), k≤2k\leq2. This follows by reversing (E7) for first derivatives and then applying it again; derivatives of the sphere factors are bounded. Using (E15), t−Tt-T bounded, and (E67), we conclude eqT𝒟kU∈L2((T1,∞)×Sn−1)(q∈ℝ,0≤k≤2).(E68) e^{qT}\mathcal D^kU\in L^2((T_1,\infty)\times S^{n-1}) \quad(q\in\mathbb R,\ 0\leq k\leq2). \tag{E68} For instance, the measure conversion for the kk-th Cartesian contribution changes a squared exponential weight e2qTe^{2qT} into a fixed radial power comparable to r2q+2k−nr^{2q+2k-n}; (E67) allows every such power. This checks the Jacobian, rather than inferring (E68) from a pointwise assertion of decay.

Fix T0T_0 above the thresholds used in the Carleman estimate. Choose a real smooth cutoff χ\chi, zero for T≤T0+1T\leq T_0+1 and one for T≥T0+2T\geq T_0+2. Let θL\theta_L be one for T≤LT\leq L, zero for T≥L+1T\geq L+1, with first two derivatives bounded independently of LL. Apply (E64), by its H2H^2 extension, to UL=χθLU.(E69) U_L=\chi\theta_LU. \tag{E69} For a fixed τ\tau, (E68) permits L→∞L\to\infty in every term. In detail, all upper-cutoff commutators are supported in [L,L+1][L,L+1] and are bounded by C(|U|+|𝒟1U|)C(|U|+|\mathcal D^1U|), since the potential commutes and QQ has bounded differential coefficients. Their weighted L2L^2 norms tend to zero by (E68). Equation (E14) makes eτTQUe^{\tau T}QU square integrable, so the noncommutator terms converge as well. Derivatives on the left converge by the same argument. Thus (E64) holds for χU\chi U. Smoothing occurs first for each compactly supported ULU_L, then L→∞L\to\infty at fixed τ\tau, and only later will τ→∞\tau\to\infty.

Write Sτ(W)=∥e(τ+1)TW∥2+∥eτT𝒟1W∥2,m0=e−T0/2+τ−1. S_\tau(W)=\|e^{(\tau+1)T}W\|^2 +\|e^{\tau T}\mathcal D^1W\|^2,\qquad m_0=e^{-T_0/2}+\tau^{-1}. Using (E14), the product rule, and χ𝒟U=𝒟(χU)−(𝒟χ)U\chi\mathcal D U=\mathcal D(\chi U)-(\mathcal D\chi)U, we obtain ∥eτTQ(χU)∥2≤C1Sτ(χU)+C2e2τ(T0+2)H02.(E70) \|e^{\tau T}Q(\chi U)\|^2 \leq C_1 S_\tau(\chi U)+C_2e^{2\tau(T_0+2)}H_0^2. \tag{E70} Here H0H_0 is a fixed finite norm of U,𝒟1UU,\mathcal D^1U on the transition strip [T0+1,T0+2][T_0+1,T_0+2], with any fixed bounded weight such as eTe^T included. It is independent of τ\tau. The constants controlling the equation near infinity are uniform in the strip position once the initial threshold is fixed.

By (E64) and (E70), Sτ(χU)≤Cm0C1Sτ(χU)+Cm0C2e2τ(T0+2)H02. S_\tau(\chi U)\leq C m_0 C_1 S_\tau(\chi U) +C m_0 C_2e^{2\tau(T_0+2)}H_0^2. Increase the fixed T0T_0, then the lower threshold for τ\tau, until CC1m0≤1/2CC_1m_0\leq1/2. Absorb the first right-side term. For each fixed σ>0\sigma>0, restrict the zeroth-order norm to T>T0+2+σT>T_0+2+\sigma, where χ=1\chi=1, to deduce ∥eTU∥L2(T>T0+2+σ)2≤Cm0e−2τσH02.(E71) \|e^TU\|_{L^2(T>T_0+2+\sigma)}^2 \leq C m_0e^{-2\tau\sigma}H_0^2. \tag{E71} Let τ→∞\tau\to\infty. The right side tends to zero with T0,σT_0,\sigma fixed. Taking a countable union of these regions as σ↓0\sigma\downarrow0 proves U=0U=0 for T>T0+2T>T_0+2. We have obtained a nonempty exterior open zero set for uu.

It remains to justify continuation throughout XX. In dimensions greater than two, Section 8 of Curved weights and the directions in which support can end says that every real normal is admissible for every elliptic complex quadratic form. In dimension two, choose independent real covectors ξ,N\xi,N. The two roots of z↦px(ξ+zN)(E72) z\longmapsto p_x(\xi+zN) \tag{E72} cannot cross the real axis as xx varies, by ellipticity, and their upper-half-plane count is locally constant. Far out, Re⁡px\operatorname{Re}p_x is positive definite. The path Re⁡px+isIm⁡px\operatorname{Re}p_x+i s\operatorname{Im}p_x, 0≤s≤10\leq s\leq1, stays elliptic. At s=0s=0 its roots are a nonreal conjugate pair, so the upper count is one also at s=1s=1. Connectedness of XX makes the same count equal to one everywhere. Thus a double nonreal root never occurs, and every real normal is admissible throughout XX. This argument uses asymptotic positivity; it does not assert that ajk(x)a_{jk}(x) are real at some finite point.

On X\{0}X\setminus\{0\}, the local equation has bounded lower-order coefficients on compact sets. Section 7 of Curved weights and the directions in which support can end therefore excludes every normal to a proper support boundary. Its open-set propagation consequence gives u=0u=0 on this domain. When n≥2n\geq2, removing one point from a connected open set leaves it connected: a polygonal path can be modified inside a sufficiently small ball about the removed point by an arc on a sphere, without leaving the open set. If 0∈X0\in X, its singleton is a null set, so vanishing off zero proves the asserted almost-everywhere conclusion on XX.

For n=1n=1, a connected open neighborhood of both ends of the line is the whole line. Interpret S0S^0 as its two points, with counting measure; the angular fields and their sums are zero. The polar identity is ∂t2−∂t\partial_t^2-\partial_t, which is (E9) for n=1n=1. All estimates above remain valid on the two half-cylinders. The Fourier shell in Section 4 is empty in this case; its off-shell estimate suffices. The proof of (E52) used only boundedness of cc and c′c', so also applies. The two exterior tails vanish. In dimension one a nonzero quadratic symbol has no exceptional nonzero normal, by Section 8 of Curved weights and the directions in which support can end. Propagate from the two tails on the two components of X\{0}X\setminus\{0\}, and ignore the null singleton. The same reasoning proves a one-ended version on a half-line which avoids the origin; if a half-line crosses zero, propagation across it needs a locally bounded differential inequality there. The singular inequality (E5) alone does not supply that additional conclusion. This completes the theorem in every dimension. ▫\square

12.1. Polynomial weights on one tail suffice for the solution alone

The proof of Section 12 uses weighted norms only on an exterior region. Its first-derivative assumption follows from an energy estimate there. We prove that implication without assuming global integrability near a finite boundary of the original domain.

Corollary. Retain (E1)–(E3), λ>0\lambda>0, u∈Hloc1(X)u\in H^1_{\mathrm{loc}}(X), the inequality (E5) near infinity, and the locally bounded continuation inequality on compact subsets of X\{0}X\setminus\{0\}. In place of (E4), it suffices to assume, for one exterior radius RuR_u, (1+|x|)su∈L2({|x|>Ru})for every real s.(ECT1) (1+|x|)^s u\in L^2(\{|x|>R_u\}) \quad\text{for every real }s. \tag{ECT1} Then the original solution vanishes almost everywhere on XX. The two-ended dimension-one formulation and the qualification for a half-line crossing zero remain exactly those in Section 12. For the full real definite limiting matrix (E3a), the same conclusion holds with the original required energy sign σλ>0\sigma\lambda>0. No all-weight derivative assumption, or global integrability approaching a finite boundary of XX, is required.

Coercivity of the full complex matrix on a large annulus. Select R0≥1R_0\geq1 so large that, for every R≥R0R\geq R_0, the closure of AR′={R/2<|x|<4R} A_R'=\{R/2<|x|<4R\} lies inside the region where (E3) and (E5) hold and inside XX. Increase R0R_0 to ensure nCa(R0/2)−1−δ≤1/2nC_a(R_0/2)^{-1-\delta}\leq1/2. The entrywise bound gives ∥A−I∥op≤nmax⁡j,k|ajk−δjk|≤1/2\|A-I\|_{\mathrm{op}}\leq n\max_{j,k}|a_{jk}-\delta_{jk}|\leq1/2. Indeed for a complex vector zz, each component of (A−I)z(A-I)z has absolute value at most the entry maximum times ∑k|zk|≤n|z|\sum_k|z_k|\leq\sqrt n|z|; summing its nn component squares proves the displayed norm bound. Consequently Re⁡∑j,kajkzkzj¯≥12|z|2,∥A∥op≤32(x∈AR′,z∈ℂn).(ECT2) \operatorname{Re}\sum_{j,k}a_{jk}z_k\overline{z_j} \geq\tfrac12|z|^2,\qquad \|A\|_{\mathrm{op}}\leq\tfrac32 \quad(x\in A_R',\ z\in\mathbb C^n). \tag{ECT2} This uses the full complex sesquilinear expression. Positivity on complex vectors has not been inferred merely from the real-covector ellipticity assumption.

The full annular energy identity. Choose a real smooth cutoff χ0\chi_0, with 0≤χ0≤10\leq\chi_0\leq1, equal to one on 1≤|y|≤21\leq|y|\leq2, compactly supported in 1/2<|y|<41/2<|y|<4, and put Cχ=∥∇χ0∥∞C_\chi=\|\nabla\chi_0\|_\infty. Set χR(x)=χ0(x/R)\chi_R(x)=\chi_0(x/R), AR={R<|x|<2R}A_R=\{R<|x|<2R\}, and retain q=(pA−λ)u,bk=∑j∂jajk,bR=n3/2Ca(R/2)−2−δ,|b(x)|≤bR,|q(x)|≤(2C/R)(|u(x)|+|∇u(x)|),U=∥u∥L2(AR′),G=∥χR∇u∥2,H=∥u∇χR∥2≤CχU/R.(ECT3) \begin{gathered} q=(p_A-\lambda)u,\qquad b_k=\sum_j\partial_j a_{jk},\\ b_R=n^{3/2}C_a(R/2)^{-2-\delta},\qquad |b(x)|\leq b_R,\quad |q(x)|\leq(2C/R)(|u(x)|+|\nabla u(x)|),\\ U=\|u\|_{L^2(A_R')},\quad G=\|\chi_R\nabla u\|_2,\quad H=\|u\nabla\chi_R\|_2\leq C_\chi U/R. \end{gathered} \tag{ECT3} The coefficient n3/2n^{3/2} follows by bounding each of the nn terms in each bkb_k by Ca(R/2)−2−δC_a(R/2)^{-2-\delta}, and then taking the Euclidean norm of its nn components. On the cutoff support, the original inequality and local H1H^1 regularity give pAu∈L2p_Au\in L^2. Sections 7–8 of Local inverses and distance-weighted elliptic estimates give H2H^2 on a neighborhood of that support. The weak integration identity can therefore be proved by H2H^2 approximation and the Lipschitz product rule. Its exact nondivergence form is ∫(pAu)χR2u‾=∑j,k∫ajk∂ku(χR2∂ju‾+2χR(∂jχR)u‾)+∑k∫bk∂kuχR2u‾.(ECT4) \begin{split} \int(p_Au)\chi_R^2\bar u ={}&\sum_{j,k}\int a_{jk}\partial_k u \bigl(\chi_R^2\partial_j\bar u +2\chi_R(\partial_j\chi_R)\bar u\bigr)\\ &+\sum_k\int b_k\partial_k u\,\chi_R^2\bar u. \end{split} \tag{ECT4} All integrals are over the cutoff support, extended by zero outside it. The plus signs result from pA=−∑ajk∂j∂kp_A=-\sum a_{jk}\partial_j\partial_k, with one integration by parts in xjx_j. The original full skew entries, their derivative contribution to bb, and both cutoff terms remain in this identity.

Take real parts and use pAu=λu+qp_Au=\lambda u+q, (ECT2), Cauchy–Schwarz, and 0≤χR≤10\leq\chi_R\leq1. The equation term is bounded by (λ+2C/R)U2+(2C/R)GU(\lambda+2C/R)U^2+(2C/R)GU. The coefficient derivative term is bounded by bRGUb_RGU. The cutoff cross term is bounded by 2∥A∥opGH≤3GH2\|A\|_{\mathrm{op}}GH\leq3GH. Thus 12G2≤(λ+2C/R)U2+LRGU,LR=(2C+3Cχ)/R+bR.(ECT5) \tfrac12G^2\leq(\lambda+2C/R)U^2+L_RGU, \qquad L_R=(2C+3C_\chi)/R+b_R. \tag{ECT5} The exact inequality LRGU≤G2/4+LR2U2L_RGU\leq G^2/4+L_R^2U^2 follows by squaring G/2−LRUG/2-L_RU. Since χR=1\chi_R=1 on ARA_R, it yields ∥∇u∥L2(AR)2≤G2≤4(λ+2C/R+LR2)∥u∥L2(AR′)2.(ECT6) \|\nabla u\|_{L^2(A_R)}^2\leq G^2 \leq4\bigl(\lambda+2C/R+L_R^2\bigr) \|u\|_{L^2(A_R')}^2. \tag{ECT6} Every term of LRL_R decreases for R≥R0R\geq R_0. We therefore have the explicit common finite bound Cext=4(λ+2C/R0+LR02)(ECT7) C_{\mathrm{ext}}=4\bigl(\lambda+2C/R_0+L_{R_0}^2\bigr) \tag{ECT7} for the entire right coefficient. No weighted derivative assumption entered the proof.

Every weighted gradient tail follows. For s∈ℝs\in\mathbb R, the ratio of the maximum of (1+r)2s(1+r)^{2s} on R<r<2RR<r<2R to its minimum on R/2<r<4RR/2<r<4R is at most 62|s|6^{2|s|}. For s≥0s\geq0, use (1+2R)/(1+R/2)≤4(1+2R)/(1+R/2)\leq4; for s<0s<0, use (1+4R)/(1+R)≤4(1+4R)/(1+R)\leq4. Both are in particular at most six, and the sign of ss determines which endpoint is the maximum. Multiplying (ECT6) by that maximum gives the full comparison ∫AR(1+|x|)2s|∇u|2dx≤Cext62|s|∫AR′(1+|x|)2s|u|2dx.(ECT8) \int_{A_R}(1+|x|)^{2s}|\nabla u|^2dx \leq C_{\mathrm{ext}}6^{2|s|} \int_{A_R'}(1+|x|)^{2s}|u|^2dx. \tag{ECT8} Use R=2kR0R=2^kR_0, k≥0k\geq0. The annuli ARA_R cover |x|>R0|x|>R_0 up to their sphere boundaries, which have Lebesgue measure zero. For a given positive radius, membership in an enlarged annulus requires k−1<log⁡2(r/R0)<k+2k-1<\log_2(r/R_0)<k+2; at most four integer indices meet this condition. All these enlarged annuli lie in |x|>R0/2|x|>R_0/2. Summing nonnegative integrals therefore proves ∫|x|>R0(1+|x|)2s|∇u|2dx≤4Cext62|s|∫|x|>R0/2(1+|x|)2s|u|2dx<∞.(ECT9) \int_{|x|>R_0}(1+|x|)^{2s}|\nabla u|^2dx \leq4C_{\mathrm{ext}}6^{2|s|} \int_{|x|>R_0/2}(1+|x|)^{2s}|u|^2dx<\infty. \tag{ECT9} The right integral is finite by (ECT1) outside the larger of RuR_u and R0/2R_0/2. The intervening closed bounded annulus is compactly contained in XX, and its weight is bounded, so local H1H^1 supplies its finite integral. This is a local argument on a compact subset, not an assumption of integrability near an arbitrary finite boundary of XX.

Now (E65)–(E66) use only the original solution and first-derivative norms on those enlarged exterior annuli. They give every second-derivative tail weight (E67), and the full radial Jacobian gives every cylinder weight (E68). The entire cutoff argument (E69)–(E71) consequently applies, with its original order of limits, to obtain the same exterior open zero set. The root-count and compact-set continuation argument (E72), including its dimension-one qualifications, then gives u=0u=0 almost everywhere on the original XX. This proves the corollary without invoking the preceding theorem under an unmet global version of (E4). ▫\square

Returning a full definite limiting matrix. Keep every datum in (E3a)–(E3f). The exact auxiliary field is Ã=σM−1A(My)M−T\widetilde A=\sigma M^{-1}A(My)M^{-T}, with limit I+K∞I+K_\infty, rather than II. Introduce its symmetric part B̃=(Ã+ÃT)/2\widetilde B=(\widetilde A+\widetilde A^T)/2 for the energy estimate. Formulas (E2a) and (E8a), with the same weak product argument as (ECT4), prove pB̃=pÃp_{\widetilde B}=p_{\widetilde A} on punctured compact sets. Its limit is exactly II. The full entry and derivative comparisons in (E3d) give its two required decay bounds, since averaging a pair of entries retains those bounds with their displayed matrix sums. Apply (ECT2)–(ECT9) to this auxiliary symmetric field and positive energy λ̃=σλ\widetilde\lambda=\sigma\lambda, retaining the exact inequality (E3e).

The original solution tail (ECT1) transfers to v=u∘Mv=u\circ M by the actual singular-value inequalities in (E3f). Choose the auxiliary threshold large enough that m−R0/2m_-R_0/2 exceeds every original coefficient, equation and domain threshold. For each exterior radius RR, the exact restricted measure and gradient identity is ∫|y|>R(1+|My|)2s(|v|2+|M−TDyv|2)dy=|det⁡M|−1∫|M−1x|>R(1+|x|)2s(|u|2+|Dxu|2)dx.(ECT10) \begin{split} &\int_{|y|>R}(1+|My|)^{2s} \bigl(|v|^2+|M^{-T}D_yv|^2\bigr)\,dy\\ &\qquad=|\det M|^{-1} \int_{|M^{-1}x|>R}(1+|x|)^{2s} \bigl(|u|^2+|D_xu|^2\bigr)\,dx. \end{split} \tag{ECT10} The inverse gradient entries and both singular-value weight constants in (E3f) show its finiteness after (ECT9). The region |x|>m+R|x|>m_+R is contained in |M−1x|>R|M^{-1}x|>R, so it supplies an actual original radial gradient tail as well. Sections 2–12 then return the exterior zero set through the complete maps (E77)–(E80). All original skew data, the sign σ\sigma, energy λ\lambda, gradient M−TDyvM^{-T}D_yv, integration regions and determinant remain explicit.

Equivalent tests for the weight quantifier. It is enough to test (ECT1) on any real sequence sls_l tending to +∞+\infty, including the nonnegative integers. For a fixed real ss, select sl≥ss_l\geq s. Since 1+|x|≥11+|x|\geq1, the exact inequality (1+|x|)2s≤(1+|x|)2sl(1+|x|)^{2s}\leq(1+|x|)^{2s_l} bounds the required squared integral by that tested one. Conversely all real weights include every selected sequence. This proves the equivalence for the original solution and, after (ECT9), its derivative tail, without changing their measures or domains.

The exact inner and enlarged annuli used for the exterior energy estimate

The drawing is a two-dimensional section of the nn-dimensional supports in (ECT3)–(ECT9), with all four radii in their actual ratio. Its displayed cutoff is the exact function h(t)={e−1/t,t>0,0,t≤0,η(t)=h(t)h(t)+h(1−t),χ0(y)=η(4|y|−3)η((7−2|y|)/3).(ECT11) \begin{gathered} h(t)=\begin{cases}e^{-1/t},&t>0,\\0,&t\leq0,\end{cases} \qquad \eta(t)=\frac{h(t)}{h(t)+h(1-t)},\\ \chi_0(y)=\eta(4|y|-3)\eta\bigl((7-2|y|)/3\bigr). \end{gathered} \tag{ECT11} The denominator is everywhere positive. Repeated derivatives of hh on the positive ray are a finite polynomial in t−1t^{-1} times e−1/te^{-1/t}; they all tend to zero at zero. Thus hh and η\eta are smooth, with η=0\eta=0 on t≤0t\leq0 and η=1\eta=1 on t≥1t\geq1. This χ0\chi_0 is zero for |y|≤3/4|y|\leq3/4 and |y|≥7/2|y|\geq7/2, equals one for 1≤|y|≤21\leq|y|\leq2, and is smooth even at the origin because it vanishes in a neighborhood there. Its support is compactly contained in the enlarged annulus, and its smooth gradient has finite maximum CχC_\chi. This verifies every cutoff property used in (ECT3) for the actual drawing.

This annular argument is a consequence of the complete exterior proof here. The original theorem and its solutions remain intact. In particular the outgoing wave (E75) still fails the required all-weight condition on the solution itself, and the negative-energy example (E74) still prevents deletion of the energy sign.

13. Worked models and precise nonconclusions

A complex angular perturbation at the allowed regularity. Let B(ω)B(\omega) be a real symmetric matrix with Lipschitz entries on the sphere, and put, on r>2r>2, a(x)=I+ir−1−δB(x/r).(E73) a(x)=I+i r^{-1-\delta}B(x/r). \tag{E73} For real ξ\xi, Re⁡(ξtaξ)=|ξ|2\operatorname{Re}(\xi^ta\xi)=|\xi|^2, so ellipticity is immediate, independently of the size of BB. Radial differentiation of r−1−δr^{-1-\delta} gives O(r−2−δ)O(r^{-2-\delta}), and angular differentiation of B(x/r)B(x/r) introduces one factor r−1r^{-1}. Thus (E3) holds almost everywhere. If measurable lower-order coefficients satisfy |β(x)|+|γ(x)|≤C/r, |\beta(x)|+|\gamma(x)|\leq C/r, then every solution of (p+β⋅D+γ−λ)u=0 (p+\beta\cdot D+\gamma-\lambda)u=0 at the stated weak H1H^1 regularity satisfies (E5). For λ>0\lambda>0, (E4) forces that solution to vanish. This example allows genuinely complex leading coefficients and merely Lipschitz angular dependence. It does not use a self-adjoint realization of the operator.

The sign of the energy changes the answer. In dimension three, set u(x)=e−κ|x||x|,|x|>2,κ>0.(E74) u(x)=\frac{e^{-\kappa|x|}}{|x|}, \qquad |x|>2,\quad \kappa>0. \tag{E74} For a radial function f(r)f(r), Δf=f″+2f′/r\Delta f=f''+2f'/r. Here f′=−e−κr(κ/r+1/r2),f″=e−κr(κ2/r+2κ/r2+2/r3), f'=-e^{-\kappa r}(\kappa/r+1/r^2),\qquad f''=e^{-\kappa r}(\kappa^2/r+2\kappa/r^2+2/r^3), so Δu=κ2u\Delta u=\kappa^2u. Therefore (−Δ−λ)u=0(-\Delta-\lambda)u=0 with λ=−κ2\lambda=-\kappa^2, and u,Duu,Du belong to every polynomially weighted L2L^2 space on the exterior. The function is nonzero. Equivalently, for the negative-definite symbol of p=Δp=\Delta, the same function solves (p−κ2)u=0(p-\kappa^2)u=0 at positive energy. Thus the relative sign cannot be discarded when comparing a general real elliptic limiting quadratic form with its auxiliary expression.

A polynomially weighted solution which does not satisfy all weights. Still in dimension three, let u(x)=eik|x||x|,|x|>2,k>0.(E75) u(x)=\frac{e^{ik|x|}}{|x|}, \qquad |x|>2,\quad k>0. \tag{E75} The same radial calculation, with κ=−ik\kappa=-ik, gives (−Δ−k2)u=0(-\Delta-k^2)u=0. Since |u|=r−1|u|=r^{-1} and |u′|2=k2r−2+r−4|u'|^2=k^2r^{-2}+r^{-4}, both weighted integrals for uu and DuDu behave at infinity like ∫2∞r2sdr\int_2^\infty r^{2s}\,dr. They are finite exactly when s<−1/2s<-1/2. This provides many weighted L2L^2 conditions, but not (E4); there is no contradiction with the theorem.

Small values do not control coefficient derivatives. Consider a(x)=(1+ir−1−δsin⁡(r3))I(r>2).(E76) a(x)=\bigl(1+i r^{-1-\delta}\sin(r^3)\bigr)I \quad(r>2). \tag{E76} Its real part is the identity and its distance from II satisfies the first bound in (E3). Its radial derivative contains 3ir1−δcos⁡(r3)3i r^{1-\delta}\cos(r^3), so the second bound in (E3) fails. The theorem has not been proved under only the first bound. This example identifies a missing assumption in an attempted application; it is not a counterexample to a more general uniqueness theorem.

These examples isolate four different issues: complex coefficients, the sign of the limiting form relative to the energy, quantification over all weights, and independent control of first coefficient derivatives.

14. Problems with complete solutions

Problem 1: anisotropy and the unchanged decay exponents. In ℝ3\mathbb R^3, suppose the coefficient matrix tends to G=diag⁡(4,1,9)G=\operatorname{diag}(4,1,9) with the two rates in (E3). Find the full linear coordinate comparison, retain the original matrix and Jacobian, and determine the energy sign required by the theorem.

Solution. Put x=(2y1,y2,3y3)x=(2y_1,y_2,3y_3), so S=G1/2=diag⁡(2,1,3)S=G^{1/2}=\operatorname{diag}(2,1,3). The chain rule gives Dx=S−tDyD_x=S^{-t}D_y; hence the new coefficient matrix is ã(y)=S−1a(Sy)S−t. \widetilde a(y)=S^{-1}a(Sy)S^{-t}. Its limit is S−1GS−t=IS^{-1}GS^{-t}=I. Since |y|≤|Sy|≤3|y||y|\leq|Sy|\leq3|y|, the error is O(|y|−1−δ)O(|y|^{-1-\delta}). Differentiating a(Sy)a(Sy) introduces only a fixed matrix factor, giving O(|y|−2−δ)O(|y|^{-2-\delta}). The Jacobian is the constant det⁡S=6\det S=6. Formula (E3f), with m−=1,m+=3m_-=1,m_+=3, gives the exact weighted integral and both comparisons for every real exponent. Formula (E79) retains that factor six, every radial and hh factor, and the original p−λp-\lambda in its original coordinates; (E80) supplies every original derivative. The spectral parameter is unchanged because the change of variables has not multiplied the equation by a scalar. Thus the required sign is λ>0\lambda>0. If the limit were −G-G, multiplication by −1-1 would replace the energy by −λ-\lambda; the theorem would require the original λ<0\lambda<0.

Problem 2: locate the three regimes without losing a parameter. Take A≥1A\geq1, η=1/2\eta=1/2, and τ=Aq\tau=A^q with q>0q>0. Compute the choice (E31), identify both transition exponents, and check K≥AK\geq A.

Solution. For A>1A>1, the conditions τ2≤A2\tau^2\leq A^2 and τ2≥A2+η\tau^2\geq A^{2+\eta} become q≤1q\leq1 and q≥5/4q\geq5/4. When A=1A=1, one has τ=K=1\tau=K=1, and all the expressions agree for every qq. For A>1A>1 the regimes give K={A2−q,0<q≤1,A3q−2,1≤q≤5/4,Aq+1/2,q≥5/4. K= \begin{cases} A^{2-q},&0<q\leq1,\\ A^{3q-2},&1\leq q\leq5/4,\\ A^{q+1/2},&q\geq5/4. \end{cases} At q=1q=1, the first two exponents are both one. At q=5/4q=5/4, the last two exponents are both 7/47/4. Every exponent is at least one in its designated range, proving K≥AK\geq A. Moreover τA2/K\tau A^2/K equals A2qA^{2q}, A4−2qA^{4-2q}, and A3/2A^{3/2}, respectively. The middle exponent is at least 3/23/2, which checks the condition M2K≤τA2M^2K\leq\tau A^2 when M≤min⁡(A3/4,τ)M\leq\min(A^{3/4},\tau).

Problem 3: why the second-derivative error has its stated weight. Bound Ij=∫e−(1+d)Tτj|𝒟2V||𝒟sV|,j+s≤1, I_j=\int e^{-(1+d)T}\tau^j|\mathcal D^2V|\,|\mathcal D^sV|, \qquad j+s\leq1, by R(V)R(V). Explain why replacing its first term by an unweighted H1H^1 norm does not follow from the same argument.

Solution. Factor the integrand as in (E20) and apply 2ab≤a2+b22ab\leq a^2+b^2: Ij≤12τ−1∥e−T𝒟2V∥2+12τ2j+1∥e−dT𝒟sV∥2. I_j\leq\tfrac12\tau^{-1}\|e^{-T}\mathcal D^2V\|^2 +\tfrac12\tau^{2j+1}\|e^{-dT}\mathcal D^sV\|^2. Since 2j+1≤3−2s2j+1\leq3-2s, the second term is at most half the corresponding term in RR. The first term is exactly its order-two term. There is no pointwise or unrestricted norm inequality bounding two derivatives by one derivative. For example a fixed compactly supported amplitude multiplied by eiky1e^{iky_1} in a chart has second-derivative norm growing like k2k^2, while its first-derivative norm grows like kk. The separate Fourier estimate, involving QτVQ_\tau V, is what eventually controls that order-two contribution.

Problem 4: a lower limit for the shell parameter. Assume (E24) and (E30). Prove the necessary lower bound (E35), and explain why τ3/A2\tau^3/A^2 cannot be used for KK in all three regions.

Solution. Rearranging the second inequality of (E24) gives K≥τ3/(A−ητ2+A2)K\geq\tau^3/(A^{-\eta}\tau^2+A^2); (E30) gives K≥A2/τK\geq A^2/\tau. Their maximum is (E35). If K=τ3/A2K=\tau^3/A^2 and τ<A\tau<A, then A2/K=A4/τ3>τA^2/K=A^4/\tau^3>\tau, violating (E30). If τ2>2A2+η\tau^2>2A^{2+\eta}, then A−ητ2>2A2=τ3/K+A2A^{-\eta}\tau^2>2A^2=\tau^3/K+A^2, violating the first inequality in (E24). Thus the middle expression fails in both sufficiently extreme regions, for two different reasons.

Problem 5: the endpoint cutoff limit and its order. Suppose only (E68) and (E14) are known, and χ,θL\chi,\theta_L are as in (E69). Show that the upper-cutoff error disappears for each fixed τ\tau, and explain why this is not a uniform statement as τ→∞\tau\to\infty.

Solution. Every derivative of θL\theta_L is supported in [L,L+1][L,L+1], with a bound independent of LL. Since the coefficients of the differential part of QQ are bounded, the product rule gives ∥eτT[Q,θL](χU)∥≤C∥eτT(|U|+|𝒟1U|)∥L2(L<T<L+1) \|e^{\tau T}[Q,\theta_L](\chi U)\| \leq C\|e^{\tau T}(|U|+|\mathcal D^1U|)\|_{L^2(L<T<L+1)} for L>T0+3L>T_0+3. The right side tends to zero as a tail of a fixed L2L^2 function, by (E68). The potential contributes no commutator. Also eτTQU∈L2e^{\tau T}QU\in L^2 by (E14) and the q=τ+1,τq=\tau+1,\tau cases of (E68), so multiplication by θL\theta_L converges on the equation term. Nothing in (E68) bounds the norms uniformly over all qq; the constants may grow arbitrarily with qq. Therefore the justified order is smoothing on a fixed compact set, removing the upper cutoff at fixed τ\tau, and then sending τ\tau to infinity in the already established estimate.

Problem 6: propagation without a real coefficient point. Suppose n=2n=2, XX is connected, the quadratic principal forms are continuous and elliptic, and their real parts are positive definite at one point. Prove that every line polynomial (E72), with independent real ξ,N\xi,N, has one root in each open half-plane throughout XX. Explain the consequence for a locally Lipschitz equation which vanishes on an exterior open set.

Solution. At the selected point, the path that multiplies the imaginary part of the form by s∈[0,1]s\in[0,1] keeps its positive real part and hence remains elliptic. At s=0s=0, the real quadratic polynomial in the line parameter has no real roots and therefore has a conjugate pair. The upper-half-plane count is one. A root cannot cross the real axis along this path, so the same count holds for the original complex form at that point. For a fixed independent pair ξ,N\xi,N, continuity of the unordered two-root set, including multiplicities, follows from the quadratic formula. Ellipticity prevents real roots everywhere in XX, and the leading coefficient px(N)p_x(N) never vanishes. Consequently the upper count is locally constant and hence constant on connected XX. It remains one. The roots are distinct, since a double root would put both in one half-plane. The same argument applies to every independent pair; dependent pairs only give the zero complex vector excluded from the exceptional-normal definition. Thus the exceptional normal set is empty. Section 7 of Curved weights and the directions in which support can end then propagates any nonempty open zero set through a connected region where the lower-order inequality has locally bounded coefficients. The proof used a point with positive real part, not a point at which all coefficients were real.

References

The proof of the asymptotically constant operator is given here; it includes the parameter and subsidiary error estimates. The sign convention and the ellipticity needed for propagation have been made explicit.

For a comparison with scattering applications, Richard Melrose’s Spectral and scattering theory for the Laplacian on asymptotically Euclidian spaces, §10, derives rapid decay by microlocal estimates and then invokes exterior uniqueness. Its use of that theorem does not replace the proof supplied here. A useful research route is to determine which coefficient and end-geometry conditions allow the two estimates above after radial compactification; the smooth scattering-metric setting in that work provides a concrete comparison.

Semyon Dyatlov and Maciej Zworski’s Mathematical Theory of Scattering Resonances, version 1.0 of August 19, 2022, Theorems 3.33 and 3.35 and Lemma 3.34, give related Rellich and Carleman arguments. The checked statements use a real compactly supported potential or a self-adjoint operator equal to the Euclidean Laplacian outside a compact set. They provide an instructive route from radiation conditions to uniqueness. They do not cover the complex Lipschitz principal perturbations with quantified decay in (E3), and are not used as a proof import for that assertion.

Eugenia Malinnikova’s Uniqueness results for solutions of continuous and discrete PDE, published in 2023, §3, surveys decay questions for bounded Schrödinger potentials. Its hypotheses and decay scales differ from the positive fixed energy and r−1r^{-1} error in (E5). Comparing the mechanisms is a research reading exercise; the results reported there do not turn (E4) into a theorem for arbitrary bounded potentials. That chapter carries CC BY 4.0.

Further questions

A further research direction is quantitative dependence on λ\lambda as λ↓0\lambda\downarrow0. The constants above may depend on λ−1\lambda^{-1}, and the proof spends a positive-potential term in both (E54) and (E60). A uniform zero-energy estimate would therefore require additional analysis. This identifies a missing extension of the present proof, not a claim that the zero-energy problem is unsolved in mathematics.