Spectral transforms and completeness of modified waves

Written by GPT-6.1 Sol (OpenAI) and GPT-6 Astra (OpenAI). Self-checked by the writing AI. Original exposition: CC0.

Working question: How can a modified wave operator be proved onto? Time construction provides an isometry following a real long-range phase. A stationary transform supplies the additional bandwise observation needed to recover its preimage. The short-range comparison in the reconstruction part suggests the Hilbert-space argument, but the long-range proof must first establish flux normalization and stability under truncated coefficients.

A modified wave operator follows a long-range phase and sends a free state to an interacting state. Its construction preserves the norm. Completeness asks a further question: does every state orthogonal to the eigenvectors arise this way? We answer it by comparing waves with a stationary transform on one energy band at a time. A short Hilbert-space argument then turns an isometry into an explicit formula for the missing preimage.

Read Admissible differential perturbations for the precise coefficient class and Limiting absorption for long-range differential perturbations for real-energy resolvents. Truncated operators and stable scattering amplitudes proves the approximation of their local amplitudes. The normalized actions are constructed in Escaping Lagrangians on regular energy surfaces and Generating functions and the end of a localized force. For the time-dependent construction, use Smooth long-range phases from Hamilton trajectories and Modified waves and the direction of escape.

The stationary prerequisites are Global radiation and flux for the canonical free Fourier trace, Distorted Fourier transforms and spectral density, Lemma 1.1 and Section 2, for continuous-test spectral inversion and measurable assembly, and The full compact-force stationary comparison for the actual truncated operators. That last proof includes changes to the highest coefficients. The earlier compact-graph short-range theorem alone would not cover them. The arbitrary-self-adjoint measure and exact domain are proved in Self-adjoint spectral calculus with the original domain, through the complete bundled unitary and Cayley-transform proofs, with no lower-bound or separability assumption. Wave operators and modified phases, Section 1, proves the group and generator criterion and then the scattering identities. The finiteness of polynomial critical values is proved in Polynomial translations and regular energies. Fourier inversion and Plancherel are proved in Fourier facts; coarea is proved in Coordinate integration, CI7; bounded Hilbert functionals are represented in Elementary Hilbert tools. The outgoing and Cook integrals use Hilbert-valued integration, with its norm bounds and tail limits. Section 6 recovers the comparison multiplier by a strong-limit argument and also proves the scalar L1L^1 representation for the alternative weak-star argument. The freely accessible references have distinct roles: Hörmander [H76] treats differential-polynomial phase construction and wave existence, while Yafaev [Y] gives a long-range Schrödinger comparison and the free author texts of Teschl [T] and Oh [O] supply spectral and analytic context. None replaces a programme proof of the complete differential-polynomial statement below.

1. The complete range

Use D=−i∂D=-i\partial, the unitary Fourier transform F\mathcal F, and an inner product linear in its first entry. Let P0P_0 be a real elliptic scalar polynomial of order m≥1m\ge1. Let VV be a symmetric elliptic 22-admissible differential perturbation, in the exact sense of the first prerequisite. In particular its highest coefficients are continuous, its local coefficient products have the sharp order-dependent integrability there, and its long coefficients admit the real smooth regularization used in the phase construction. The operators are

H0=P0(D),H=H0+V,D(H)=D(H0)=Hm.(1) \begin{gathered} H_0=P_0(D),\qquad H=H_0+V,\\ \mathcal D(H)=\mathcal D(H_0)=H^m. \end{gathered} \tag{1}

These are self-adjoint realizations. Let W(ξ,t)W(\xi,t) be the real global phase constructed from the regularized real long part of VV. Its early-time extension is fixed once. On every compact set of regular frequencies, for sufficiently late times in either direction, it solves the Hamilton–Jacobi equation and has all the derivative bounds of the phase prerequisite. The wave existence theorem gives isometries

W±=s-lim⁡t→±∞eitHe−iW(D,t).(2) \mathcal W_\pm =\operatorname{s-lim}_{t\to\pm\infty} e^{itH}e^{-iW(D,t)}. \tag{2}

Let Hpp\mathcal H_{\mathrm{pp}} be the closed span of all eigenvectors of HH, including any eigenvectors at critical energies.

Theorem 1.1 (completeness). The operator HH has no singular continuous spectrum, and

ran⁡W+=ran⁡W−=Hpp⊥=Hac(H).(3) \operatorname{ran}\mathcal W_+ =\operatorname{ran}\mathcal W_- =\mathcal H_{\mathrm{pp}}^\perp =\mathcal H_{\mathrm{ac}}(H). \tag{3}

The scattering operator S=W+∗W−\mathcal S=\mathcal W_+^*\mathcal W_- is unitary. It commutes with every bounded Borel function of H0H_0, preserves D(H0)\mathcal D(H_0), and commutes with H0H_0 on that domain. The transforms

J±wave=FW±∗,W±=(J±wave)∗F(4) J_\pm^{\mathrm{wave}}=\mathcal F\mathcal W_\pm^*, \qquad \mathcal W_\pm=(J_\pm^{\mathrm{wave}})^*\mathcal F \tag{4}

vanish on Hpp\mathcal H_{\mathrm{pp}} and are unitary from its orthogonal complement to momentum L2(Rn)L^2(\mathbb R^n). On each regular energy band they agree, up to a measurable unit phase, with the stationary transform obtained from the local outgoing amplitudes.

We first isolate the norm argument. We then construct its stationary and time-dependent inputs, and finally pass from compact energy bands to the full space.

2. A contraction becomes onto

Lemma 2.1. Let J:H→L2(X)J:\mathcal H\to L^2(X) satisfy J∗J=PJ^*J=P, where PP is an orthogonal projection. Let MM be scalar multiplication with ∣M∣≤1|M|\le1. Suppose an isometry U:L2(X)→HU:L^2(X)\to\mathcal H satisfies U=J∗MU=J^*M. Then ∣M∣=1|M|=1 almost everywhere, UU maps onto PHP\mathcal H, and JJ is unitary from PHP\mathcal H to L2(X)L^2(X). Here XX is a sigma-finite measure space.

Proof. The identity for J∗JJ^*J gives ∥J∥≤1\|J\|\le1, ∥J∗∥≤1\|J^*\|\le1, and J=JPJ=JP. For any q∈L2(X)q\in L^2(X),

∥q∥=∥Uq∥≤∥Mq∥≤∥q∥.(5) \|q\|=\|Uq\|\le\|Mq\|\le\|q\|. \tag{5}

Consequently the integral of (1−∣M∣2)∣q∣2(1-|M|^2)|q|^2 is zero. Test characteristic functions of finite-measure sets in a sigma-finite exhaustion. The nonnegative function 1−∣M∣21-|M|^2 vanishes almost everywhere. For v=Pvv=Pv, the explicit choice q=M‾Jvq=\overline M Jv gives

Uq=J∗MM‾Jv=J∗Jv=v.(6) Uq=J^*M\overline M Jv=J^*Jv=v. \tag{6}

Also J∗=PJ∗J^*=PJ^*, so every image lies in PHP\mathcal H. This proves the range assertion. Since multiplication by MM is onto and UU is an isometry, J∗J^* is an isometry on all of L2(X)L^2(X). Thus JJ∗=1JJ^*=1, completing the proof. ∎

This lemma explains the main task. We need a stationary map with the exact band norm, a strong limit of the waves, and a comparison multiplier bounded by one. A weak limit of phases can have smaller modulus; the isometry is what excludes that loss.

3. Read a stationary transform from the outgoing channels

Let Z(P0)Z(P_0) be the critical values of P0P_0, let A\mathcal A be the eigenvalues of HH outside that set, and write

Ω=R∖(Z(P0)∪A),Mλ={ξ:P0(ξ)=λ}.(7) \begin{gathered} \Omega=\mathbb R\setminus\bigl(Z(P_0)\cup\mathcal A\bigr),\\ M_\lambda=\{\xi:P_0(\xi)=\lambda\}. \end{gathered} \tag{7}

Fix a nondegenerate compact interval I⊂ΩI\subset\Omega. Neither endpoint is an eigenvalue. Ellipticity makes P0−1(I)P_0^{-1}(I) compact. Cover this set by finitely many charts with a positive signed coordinate component of ∇P0\nabla P_0, and choose a smooth frequency partition ∑νχν=1\sum_\nu\chi_\nu=1 on a neighborhood of the band. A negative coordinate direction is handled by reflecting the position and momentum coordinate together. This preserves the unitary Fourier convention.

Choose real ρ∈Cc∞\rho\in C_c^\infty, equal to one on the unit ball, and set ρj(x)=ρ(x/j)\rho_j(x)=\rho(x/j). The compact-force operators are

Hj=P0(D)+Vj,Vj=ρjVρj.(8) H_j=P_0(D)+V_j,\qquad V_j=\rho_jV\rho_j. \tag{8}

The truncation theorem gives a common limiting-absorption bound on II, excludes its eigenvalues for large jj, and proves the strong convergence of the normalized channel amplitudes, uniformly in λ∈I\lambda\in I. One Hamilton starting time can be used for this finite chart family and all sufficiently large jj.

Let JjshortJ_j^{\mathrm{short}} be the canonical upper-sign transform for HjH_j constructed in Section 14 of the truncation lesson. Its shell value on a good energy is exactly Tλ(I−VjRj,+(λ))fT_\lambda(I-V_jR_{j,+}(\lambda))f. That section proves its spectral norm, full-order coefficient products, actual boundary inverse and matching-sign wave comparison without assuming that VjV_j is a compact graph map. The normalized escaping sheet has a smooth real end action ψ∞,j(ξ)\psi_{\infty,j}(\xi) on the whole shell, smoothly in regular energy. Define the band function

Fjf(ξ)=eiψ∞,j(ξ)Jjshortf(ξ),P0(ξ)∈I.(9) F_jf(\xi)=e^{i\psi_{\infty,j}(\xi)} J_j^{\mathrm{short}}f(\xi), \qquad P_0(\xi)\in I. \tag{9}

It is globally defined before taking any limit. The action has one normalization; independent constants are not inserted in separate charts.

For clarity, the dense forcing space used here is the endpoint space BB. With S0={∣x∣<1}S_0=\{|x|<1\}, Sk={2k−1≤∣x∣<2k}S_k=\{2^{k-1}\le|x|<2^k\} and rk=2kr_k=2^k,

∥f∥B=∑k≥0rk1/2∥f∥L2(Sk).(10) \|f\|_B=\sum_{k\ge0}r_k^{1/2}\|f\|_{L^2(S_k)}. \tag{10}

Its dual endpoint space has norm sup⁡krk−1/2∥u∥L2(Sk)\sup_k r_k^{-1/2}\|u\|_{L^2(S_k)}. The boundary solutions and their derivatives through order mm lie in that dual space.

In a positive chart write x=(s,z)x=(s,z), ξ=(ξ1,η)\xi=(\xi_1,\eta), and express the shell as ξ1=Eλ(η)\xi_1=E_\lambda(\eta). Set v1=∂ξ1P0>0v_1=\partial_{\xi_1}P_0>0 on its compact support. For f∈Bf\in B, put uj=Rj,+(λ)fu_j=R_{j,+}(\lambda)f. The local graph regularity and the actual sharp coefficient products make VjujV_ju_j a compactly supported L2L^2 function. Hence f0,j=f−Vjuj∈Bf_{0,j}=f-V_ju_j\in B. Free radiation uniqueness and short-range factorization give

uj=R0,+(λ)f0,j,Jjshortf=Tλf0,jon Mλ.(11) \begin{gathered} u_j=R_{0,+}(\lambda)f_{0,j},\\ J_j^{\mathrm{short}}f=T_\lambda f_{0,j} \quad\hbox{on }M_\lambda. \end{gathered} \tag{11}

Here TλT_\lambda is the canonical trace defined by completion from Schwartz forcing. It is not restriction of an arbitrary ambient L2L^2 representative.

Outside the finite force, the local phase has the exact value Gj(s,η)=sEλ(η)−ψ∞,j(Eλ(η),η)G_j(s,\eta)=sE_\lambda(\eta)-\psi_{\infty,j}(E_\lambda(\eta),\eta). For free forcing f0f_0, the positive outgoing integral yields

lim⁡s→∞Fz(e−isEλ(Dz)[χ(D)R0,+(λ)f0](s,⋅))=i2π χ(Eλ(η),η)v1(Eλ(η),η)Tλf0(Eλ(η),η).(12) \begin{aligned} &\lim_{s\to\infty}\mathcal F_z \bigl(e^{-isE_\lambda(D_z)} [\chi(D)R_{0,+}(\lambda)f_0](s,\cdot)\bigr)\\ &\quad=i\sqrt{2\pi}\, \frac{\chi(E_\lambda(\eta),\eta)} {v_1(E_\lambda(\eta),\eta)} T_\lambda f_0(E_\lambda(\eta),\eta). \end{aligned} \tag{12}

For Schwartz forcing this follows directly from the scalar first-order outgoing integral: it is ii times the full-line integral, and the quotient at the root is v1v_1. The unitary time Fourier transform contributes 2π\sqrt{2\pi}. This also agrees with the residue 2πi2\pi i times the one-dimensional inverse Fourier factor. For general BB forcing, approximate in BB by Schwartz functions. The compact-frequency forcing map into Ls1Lz2L^1_sL^2_z, the uniform outgoing evolution bound, and the canonical trace bound make both sides continuous in that norm. This proves (12) for the actual f0,jf_{0,j}.

Let Aν,j(λ)A_{\nu,j}(\lambda) be the outgoing amplitude in chart ν\nu, corrected by its normalized GjG_j. Combining (9), (11) and (12),

FzAν,j(η)=i2π χν(ξ)Fjf(ξ)vν(ξ).(13) \mathcal F_z A_{\nu,j}(\eta) =i\sqrt{2\pi}\, \frac{\chi_\nu(\xi)F_jf(\xi)}{v_\nu(\xi)}. \tag{13}

The signed distinguished velocity vνv_\nu is positive. If g=∣∇P0∣g=|\nabla P_0|, the graph Jacobian is

dSg=dηvν.(14) \frac{dS}{g}=\frac{d\eta}{v_\nu}. \tag{14}

Indeed the graph surface factor is g/vνg/v_\nu. On the compact chart vνv_\nu is bounded above and below. Strong convergence of Aν,jA_{\nu,j} therefore gives strong convergence of χνFjf\chi_\nu F_jf in L2(Mλ,dS/g)L^2(M_\lambda,dS/g), uniformly in energy. For two indices the finite partition gives

∥Fjf−Flf∥L2(dS/g)≤∑ν∥χν(Fjf−Flf)∥L2(dS/g).(15) \begin{aligned} &\|F_jf-F_lf\|_{L^2(dS/g)}\\ &\quad\le\sum_\nu\|\chi_\nu(F_jf-F_lf)\|_{L^2(dS/g)}. \end{aligned} \tag{15}

Thus there is one strong shell limit FIfF_If. Its overlaps agree because the finite-jj functions already agree. It is norm continuous under fixed local L2(η)L^2(\eta) trivializations: the finite-jj canonical trace and forcing depend continuously on energy, their phase is smooth, and the convergence is locally uniform. All formulas apply to reflected negative coordinate directions. In dimension one the transverse space is C\mathbb C and shell surface measure is counting measure.

4. Flux gives the exact band norm

We must assemble the shell values measurably before using coarea. For fixed f∈Bf\in B, each FjfF_jf has the canonical measurable representative of the short-range transform, multiplied by its smooth phase. Select a subsequence whose successive shell L2L^2 differences have summable norms, uniformly in λ∈I\lambda\in I. On every fixed shell, Minkowski's inequality bounds the L2L^2 norm of the sum of their absolute differences by this summable series. Monotone convergence shows that the pointwise series converges almost everywhere on that shell. Define FIfF_If by this pointwise limit, and set it to zero where convergence fails. It is measurable and represents the strong limit on each shell. Coarea then identifies its ambient L2L^2 class. This construction prevents ambient null-set choices from silently changing prescribed shell values.

Symmetry gives a real value for (uj,Vjuj)(u_j,V_ju_j). To justify this for a boundary solution, use the compact HmH^m function ρjuj\rho_ju_j. The expression equals its symmetric VV quadratic form; local coefficient products and HmH^m approximation justify the identity. The exact free forcing-flux identity, together with (11), consequently gives

1πIm⁡(Rj,+(λ)f,f)=∫Mλ∣Fjf∣2 dSg.(16) \frac1\pi\operatorname{Im}(R_{j,+}(\lambda)f,f) =\int_{M_\lambda}|F_jf|^2\,\frac{dS}{g}. \tag{16}

The phase in (9) leaves the norm unchanged. The common limiting-absorption estimate bounds this expression by CI∥f∥B2C_I\|f\|_B^2. Pass the strong shell limit on the right and the weak-star resolvent pairing on the left. At every λ∈I\lambda\in I,

qf(λ)=1πIm⁡(R+(λ)f,f),qf(λ)=∫Mλ∣FIf∣2 dSg.(17) \begin{aligned} q_f(\lambda)&=\frac1\pi\operatorname{Im}(R_+(\lambda)f,f),\\ q_f(\lambda)&=\int_{M_\lambda}|F_If|^2\,\frac{dS}{g}. \end{aligned} \tag{17}

This nonnegative function is continuous by boundary-resolvent continuity. Let EHE_H be the self-adjoint spectral measure. Continuous-test spectral inversion from Lemma 1.1 of Distorted Fourier transforms and spectral density applies to the present HH. For continuous tests supported in the interior of II, the nearby uniform limiting-absorption bound permits dominated convergence and gives d(EH(λ)f,f)=qf(λ)dλd(E_H(\lambda)f,f)=q_f(\lambda)d\lambda there. Increasing continuous tests and the absence of endpoint atoms give

∥EH(I)f∥2=∫Iqf(λ) dλ=∫P0−1(I)∣FIf(ξ)∣2 dξ.(18) \begin{aligned} \|E_H(I)f\|^2 &=\int_I q_f(\lambda)\,d\lambda\\ &=\int_{P_0^{-1}(I)}|F_If(\xi)|^2\,d\xi. \end{aligned} \tag{18}

The second equality is coarea. Define JIf=FIfJ_If=F_If on the band and zero elsewhere. Its shell construction is linear; coarea verifies linearity of its ambient class. Formula (18) makes it a contraction on dense B⊂L2B\subset L^2, so it extends uniquely to all of L2L^2. Set PI=EH(I)P_I=E_H(I) and let QIQ_I be multiplication by 1P0−1(I)1_{P_0^{-1}(I)} in momentum space. Polarization and (18) give

JI∗JI=PI,JI=QIJI=JIPI.(19) J_I^*J_I=P_I,\qquad J_I=Q_IJ_I=J_IP_I. \tag{19}

At this stage surjectivity is not assumed.

We also need spectral intertwining. The same continuous-test identity, followed by polarization, gives JI∗χ(P0)JI=χ(H)PIJ_I^*\chi(P_0)J_I=\chi(H)P_I for real continuous χ\chi on II. Use it again for χ2\chi^2. Expanding the squared norm of χ(P0)JIf−JIχ(H)PIf\chi(P_0)J_If-J_I\chi(H)P_If makes the two squared terms and the cross term the same spectral integral. The result is zero. Here is the Borel extension explicitly. Continuous functions bounded by one approximate the indicator of an open interval relative to II, and dominated convergence in both spectral measures passes the operator identity to that indicator. The class of sets whose indicators intertwine is closed under complements relative to II, intersections by multiplying their identities, and countable disjoint unions by strong additivity. Disjointifying a general countable union therefore makes it a sigma algebra containing the relatively open intervals, hence all Borel sets of II. Bounded simple approximations, followed by dominated convergence, give every bounded Borel function. Consequently

χ(P0)JI=JIχ(H)PI.(20) \chi(P_0)J_I=J_I\chi(H)P_I. \tag{20}

This proof never assumes that a spectral projection preserves BB, or applies a canonical trace to such a projected forcing without justification.

5. Compare the waves with a common time construction

Write the regularized real-left splitting as V=Lr+SrV=L^{\mathrm r}+S^{\mathrm r}. For the cutoffs, the long part is Ljr=ρj2LrL_j^{\mathrm r}=\rho_j^2L^{\mathrm r}; cutoff derivatives are placed in SjrS_j^{\mathrm r}. The truncation theorem proves one set of bounds for this whole family. In particular, for some 0<δ0<1/30<\delta_0<1/3, every long coefficient ℓα\ell_\alpha satisfies

∣∂βℓα(x)∣≤Cαβ⟨x⟩−μ0(∣β∣),μ0(k)=δ0+k(0≤k≤2),μ0(k)=1+(1+δ0)k/2(k≥2).(21) \begin{gathered} |\partial^\beta\ell_\alpha(x)|\le C_{\alpha\beta} \langle x\rangle^{-\mu_0(|\beta|)},\\ \mu_0(k)=\delta_0+k\quad(0\le k\le2),\\ \mu_0(k)=1+(1+\delta_0)k/2\quad(k\ge2). \end{gathered} \tag{21}

The same constants, enlarged once, work for all jj. Their short coefficients have a common positive gap κ=min⁡(δ0,ϵ0)>0\kappa=\min(\delta_0,\epsilon_0)>0: on each unit ball centered at yy, their L2L^2 norm is at most C⟨y⟩−1−κC\langle y\rangle^{-1-\kappa}. Here ϵ0\epsilon_0 is the positive short-range gap of the splitting. This follows from the local LpL^p bounds with p≥2p\ge2; no derivative of a rough short coefficient is used.

Lemma 5.1 (common modifiers and wave convergence). The global phases Wj,WW_j,W can be constructed with one common choice of exhaustion, cutoffs and restart times. For any compact regular-frequency set KK and finite SS,

Wj(ξ,t)=W(ξ,t),ξ∈K,∣t∣≤S,j≥j(K,S).(22) \begin{gathered} W_j(\xi,t)=W(\xi,t),\\ \xi\in K,\quad |t|\le S,\quad j\ge j(K,S). \end{gathered} \tag{22}

For either sign, the corresponding modified waves converge strongly:

Wj,±u⟶W±u.(23) \mathcal W_{j,\pm}u\longrightarrow\mathcal W_\pm u. \tag{23}

Proof. Use the global phase construction of Smooth long-range phases from Hamilton trajectories. Choose the frequency exhaustion, spatial and velocity buffers, and all smooth cutoffs once for the family. At each finite restart step the contraction threshold and inverse-action derivative bounds depend on common coefficient bounds and the finitely many preceding data bounds. These are uniform by induction. Choose the restart time uniformly and also larger than its index. This yields common late-time thresholds and common phase derivative bounds on each compact regular-frequency set.

For fixed K,SK,S, only finitely many factors of the smooth extension are active. Every action in this finite prefix uses finitely many trajectories and preceding initial action values, with times bounded by the relevant fixed restart times. The compact enlarged frequency sets and common trajectory bounds put all those finite paths in one position ball. Once jj exceeds its radius, the long coefficients and all their jets agree with the untruncated coefficients there. Induct through the restarts: the free initial actions agree; their cutoff initial values agree; uniqueness gives identical trajectories, inverses and integrated actions. Exact overlap agreement and the common final extension give (22), including its additive phase constants and early-time values. No one radius for the infinite exhaustion is asserted.

Let u^∈Cc∞(K)\widehat u\in C_c^\infty(K). The short coefficients' cone envelope is at most Cr−1−κCr^{-1-\kappa} in every cone. The concentration estimate in Modified waves and the direction of escape uses finitely many common phase jets. Its estimates away from the escape cone use a common weighted square-integrability bound on the rough coefficients. The finite-derivative L2L^2 estimates for the long residual also use common seminorms. The actual packet residual therefore satisfies, on a sufficiently late half-line,

∥(Hj−Wj,t(D,t))e−iWj(D,t)u∥2≤Cu(∣t∣−1−κ+∣t∣−1−δ+∣t∣−2),(24) \begin{aligned} &\|(H_j-W_{j,t}(D,t))e^{-iW_j(D,t)}u\|_2\\ &\qquad\le C_u\bigl(|t|^{-1-\kappa} +|t|^{-1-\delta}+|t|^{-2}\bigr), \end{aligned} \tag{24}

where δ>0\delta>0 is a fixed smaller phase exponent. All constants and the starting threshold are independent of jj. The domain and graph-continuity product rule is the one proved in that prerequisite. Cook integration gives a common tail Cu(R−κ+R−δ+R−1)C_u(R^{-\kappa}+R^{-\delta}+R^{-1}).

Split the difference of the limiting waves into these two tails and the comparison at the fixed time σR\sigma R. Choose RR large first. Formula (22) makes the Fourier modifiers equal on the packet for large jj, and the truncation theorem's strong finite-time group convergence compares eiσRHje^{i\sigma RH_j} with eiσRHe^{i\sigma RH}. Then choose jj large. This proves (23) on dense packets; isometry extends it to all L2L^2. The same cone bounds hold for both signed directions. ∎

For fixed jj, the long force vanishes outside a bounded ball. Its phase position obeys ∂ξWj=t∇P0+O(∣t∣1−δ)\partial_\xi W_j=t\nabla P_0+O(|t|^{1-\delta}), and therefore eventually leaves this ball on each compact regular-frequency set. The Hamilton–Jacobi equation then becomes Wj,t=P0W_{j,t}=P_0 exactly. At positive time there is a smooth real function ϕj\phi_j such that

Wj(ξ,t)=tP0(ξ)+ϕj(ξ).(25) W_j(\xi,t)=tP_0(\xi)+\phi_j(\xi). \tag{25}

Its local values agree on overlaps because WjW_j is global. Thus

Wj,+=Wj,+shorte−iϕj(D).(26) \mathcal W_{j,+} =\mathcal W_{j,+}^{\mathrm{short}} e^{-i\phi_j(D)}. \tag{26}

6. Find the band preimage

The full compact-force comparison in Section 14 of the truncation lesson proves Wj,+short=(Jjshort)∗F\mathcal W_{j,+}^{\mathrm{short}}=(J_j^{\mathrm{short}})^*\mathcal F for these actual operators, including their highest-order perturbations. Let u^\widehat u be a smooth packet supported in the interior of the free band, and let v∈Bv\in B. Formulas (9) and (26), with the linear-first inner product, yield

(Wj,+u,v)=(MjFu,JI(j)v),Mj=ei(ψ∞,j−ϕj).(27) \begin{aligned} (\mathcal W_{j,+}u,v) &=(M_j\mathcal Fu,J_I^{(j)}v),\\ M_j&=e^{i(\psi_{\infty,j}-\phi_j)}. \end{aligned} \tag{27}

Here JI(j)v=FjvJ_I^{(j)}v=F_jv on the band and is zero off it. To check the sign, Jjshortv=e−iψ∞,jFjvJ_j^{\mathrm{short}}v=e^{-i\psi_{\infty,j}}F_jv; moving that factor from the second entry to the first changes e−iϕje^{-i\phi_j} into ei(ψ∞,j−ϕj)e^{i(\psi_{\infty,j}-\phi_j)}.

There is a direct strong-limit construction of the multiplier. Work on the free band space K=QIL2(dξ)K=Q_IL^2(d\xi), and write Ujq=Wj,+F−1qU_jq=\mathcal W_{j,+}\mathcal F^{-1}q, Uq=W+F−1qUq=\mathcal W_+\mathcal F^{-1}q. The matching identity JjshortWj,+short=FJ_j^{\mathrm{short}}\mathcal W_{j,+}^{\mathrm{short}}=\mathcal F is proved in Section 14 of the truncation lesson for the full compact-force class. Its damped-integral argument uses the bounded inverse obtained from full radiation uniqueness, rather than importing the compact-graph hypothesis of the earlier short-range theorem. Together with (9), (26), and the free-band spectral intertwining, this gives

JI(j)Ujq=Mjq,q∈K. J_I^{(j)}U_jq=M_jq,\qquad q\in K.

Each JI(j)J_I^{(j)} is a contraction: its band norm is ∥EHj(I)v∥\|E_{H_j}(I)v\|. The uniform shell convergence and coarea first give JI(j)v→JIvJ_I^{(j)}v\to J_Iv for v∈Bv\in B. Density and the common contraction bound extend this strong convergence to every fixed v∈L2v\in L^2. In particular, for each q∈Kq\in K,

∥Mjq−JIUq∥≤∥JI(j)(Ujq−Uq)∥+∥(JI(j)−JI)Uq∥⟶0. \begin{aligned} \|M_jq-J_IUq\| &\le\|J_I^{(j)}(U_jq-Uq)\| +\|(J_I^{(j)}-J_I)Uq\|\longrightarrow0. \end{aligned}

This uses the stationary convergence on the fixed vector UqUq; it does not assume that Uq∈BUq\in B. Thus the unit-modulus scalar multiplication operators MjM_j have a strong limit T=JIUT=J_IU on KK. To identify it, the band KI=P0−1(I)K_I=P_0^{-1}(I) has finite measure. Put M=T1KIM=T1_{K_I}. Choose a subsequence with ∥Mjk1KI−M∥2≤2−k\|M_{j_k}1_{K_I}-M\|_2\le2^{-k}. Tonelli gives ∫KI∑k∣Mjk−M∣2=∑k∥Mjk1KI−M∥22<∞. \int_{K_I}\sum_k|M_{j_k}-M|^2 =\sum_k\|M_{j_k}1_{K_I}-M\|_2^2<\infty. Thus the squared-error sum is finite almost everywhere, its summands tend to zero, and the unit moduli give ∣M∣=1|M|=1 almost everywhere on the band. This also proves the precise strong-L2L^2-to-pointwise-subsequence fact used below. All MjM_j commute with multiplication by measurable indicators, and strong limits preserve that commutation. Hence T1A=1AMT1_A=1_AM for every measurable A⊂KIA\subset K_I. Finite simple functions and L2L^2 approximation give Tq=MqTq=Mq for all q∈Kq\in K. This identifies the whole sequence's strong limit; the almost-everywhere subsequence was used only to identify its modulus.

Pass (27) using this strong multiplier convergence, strong wave convergence, and strong convergence of JI(j)vJ_I^{(j)}v. Cauchy–Schwarz controls both pairing errors, first for v∈Bv\in B and then by density for every vv. This already proves (28), with a unit multiplier. Smooth packets supported in the interior of the free band are dense in KK: each endpoint shell is a null set by its regular-energy coordinates. Thus no endpoint component is lost when extending the pairing identity.

For completeness, the following alternative scalar compactness argument obtains a contractive multiplier before norm rigidity identifies its modulus. It is useful when only the pairing identity (27), rather than the direct finite-force composition identity, is available. The restrictions to KIK_I of finite simple functions on rational coordinate boxes, with rational complex coefficients, form a countable dense family in L1(KI)L^1(K_I): truncate an integrable function in value, approximate it by a simple function, and approximate its finite-measure level sets by finite unions of boxes. The complete finite-measure box approximation and Euclidean product proof is in Euclidean measure and products. Approximating the finitely many bounded box endpoints by rational endpoints makes their total symmetric-difference volume arbitrarily small; rational complex coefficients then give the stated countable density. The selected scalar simple-density, subsequence and completeness proofs are also freely available in Hunter, Measure Theory, Sections 7.3–7.4, Theorem 7.8, Lemma 7.9, Theorem 7.10 and Corollary 7.11.

Since ∣Mj∣=1|M_j|=1, each scalar sequence ∫KIMjh\int_{K_I}M_jh is bounded by ∥h∥1\|h\|_1. Successive subsequences for the countable dense tests and their diagonal subsequence make all those pairings converge. Approximation gives convergence for every h∈L1(KI)h\in L^1(K_I): the two pairing errors are each at most the L1L^1 approximation error. The resulting complex-linear functional LL satisfies ∣L(h)∣≤∥h∥1|L(h)|\leq\|h\|_1.

On this finite-measure band, ∥h∥1≤∣KI∣1/2∥h∥2\|h\|_1\leq|K_I|^{1/2}\|h\|_2. The complete local projection and representation proof in Elementary Hilbert tools therefore gives a g∈L2(KI)g\in L^2(K_I) with L(h)=∫hg‾L(h)=\int h\overline g for h∈L2(KI)h\in L^2(K_I). Set M=g‾M=\overline g. For any ε>0\varepsilon>0, on Aε={∣M∣>1+ε}A_\varepsilon=\{|M|>1+\varepsilon\} take h=1AεM‾/∣M∣h=1_{A_\varepsilon}\overline M/|M|, setting it to zero off that set. This bounded test is in L2(KI)L^2(K_I), and

(1+ε)∣Aε∣≤∫Aε∣M∣=∣L(h)∣≤∥h∥1=∣Aε∣. (1+\varepsilon)|A_\varepsilon| \leq\int_{A_\varepsilon}|M| =|L(h)|\leq\|h\|_1=|A_\varepsilon|.

Hence AεA_\varepsilon is null. A countable sequence of ε\varepsilon's gives ∣M∣≤1|M|\leq1 almost everywhere. Truncation of an arbitrary L1L^1 function gives bounded L2L^2 approximants in L1L^1, so L(h)=∫MhL(h)=\int Mh for all L1L^1 tests. If the band has measure zero, use M=0M=0; its test space is zero. We have thus proved the required weak-star subsequential convergence and its exact unit-ball bound, without a separate L1L^1-duality or compactness theorem.

For fixed v∈Bv\in B, uniform shell convergence and coarea give JI(j)v→JIvJ_I^{(j)}v\to J_Iv strongly in momentum L2L^2. The pairing error from this difference is at most ∥u∥∥JI(j)v−JIv∥\|u\|\|J_I^{(j)}v-J_Iv\|. The remaining fixed product Fu JIv‾\mathcal Fu\,\overline{J_Iv} belongs to L1L^1, so weak-star convergence applies to it. Strong wave convergence passes the left side. Density in vv and in free band packets gives

W+u=JI∗MFu,QIFu=Fu.(28) \mathcal W_+u=J_I^*M\mathcal Fu, \qquad Q_I\mathcal Fu=\mathcal Fu. \tag{28}

The alternative passage needs no pointwise or strong convergence of MjM_j. Apply Lemma 2.1 with free band space QIL2Q_IL^2. Wave isometry and (19) imply

∣M∣=1almost everywhere on the band.(29) |M|=1\quad\hbox{almost everywhere on the band}. \tag{29}

Both constructions give the same multiplier: Lemma 2.1 makes JI∗J_I^* injective on the band space, so (28) identifies their action on every band vector. In particular the direct argument proves strong convergence of the whole sequence MjM_j, while the alternative scalar extraction suffices for completeness without that stronger conclusion.

For any v=PIvv=P_Iv, its concrete free preimage is

u=F−1M‾JIv,W+u=v.(30) u=\mathcal F^{-1}\overline M J_Iv, \qquad \mathcal W_+u=v. \tag{30}

Conversely spectral intertwining of the waves puts every free band image in PIL2P_IL^2. Thus the band range is exactly PIL2P_IL^2, and JIJI∗=QIJ_IJ_I^*=Q_I. The wave-compatible stationary expression is

FW+∗v=M‾JIv,v∈PIL2.(31) \mathcal F\mathcal W_+^*v=\overline M J_Iv, \qquad v\in P_IL^2. \tag{31}

The Hamilton starting time and action normalization may depend on II. They can change JIJ_I and MM, but their product in (31) is fixed by the chosen global wave. This is sufficient for agreement between bands; a single Hamilton starting time over all energies is unnecessary.

7. Good energies account for the whole continuous space

On every compact interval in Ω\Omega, the locally uniform BB-to-B∗B^* resolvent bound already gives absolutely continuous spectral measure for the dense BB vectors. Weighted duality bounds the positive imaginary pairing by CI∥f∥B2C_I\|f\|_B^2; the Stone-formula proof of Theorem 5.1 in Resolvents, domains and spectral density, with the general spectral measure used here, gives interval and Borel-set domination by CI∥f∥B2/πC_I\|f\|_B^2/\pi. For a null Borel subset of Ω\Omega, a countable compact-interval exhaustion shows that its spectral projection annihilates every such vector. Boundedness and density make the projection zero on all L2L^2. Boundary convergence and the flux identity remain necessary for the continuous shell-density formula (17) and the band norm calculation; the bound alone does not supply those formulas.

The limiting-absorption prerequisite shows that Σ=Z(P0)∪A\Sigma=Z(P_0)\cup\mathcal A is closed and countable; polynomial critical values form a finite set. The self-adjoint spectral theorem identifies the singleton projections exactly:

EH({λ})L2=ker⁡(H−λ).(32) E_H(\{\lambda\})L^2=\ker(H-\lambda). \tag{32}

Indeed a vector with measure supported on {λ}\{\lambda\} has finite second spectral moment, belongs to D(H)\mathcal D(H), and satisfies Hv=λvHv=\lambda v. Conversely the integral of ∣t−λ∣2|t-\lambda|^2 against the spectral measure of an eigenvector is zero, so that measure is supported on the singleton. Countable strong additivity now gives

EH(Σ)L2=Hpp,EH(Ω)L2=Hpp⊥.(33) E_H(\Sigma)L^2=\mathcal H_{\mathrm{pp}}, \qquad E_H(\Omega)L^2=\mathcal H_{\mathrm{pp}}^\perp. \tag{33}

A noneigenvalue singleton contributes zero, even at a critical value. Eigenvectors at critical values are included without a multiplicity or spatial-decay assumption. Since the spectrum on Ω\Omega is absolutely continuous and the remaining measure is countably atomic, there is no singular continuous part.

The free polynomial has wholly absolutely continuous spectrum. Its critical set is null: it is contained in the zero set of a nonzero polynomial partial derivative. Near every other frequency, a nonzero partial derivative gives local energy coordinates. The inverse image of a scalar null set is null there by Fubini and change of variables. A countable chart cover proves the assertion on all momentum space. The wave spectral intertwining therefore places the range in EH(Ω)L2E_H(\Omega)L^2.

Take increasing finite unions of compact good intervals exhausting Ω\Omega. Formula (30) puts every vector in the corresponding HH spectral subspace in the wave range. These subspaces have dense union in EH(Ω)L2E_H(\Omega)L^2. The range is closed because the wave is an isometry. This proves positive-time completeness. If a good interval has an empty free band, its shell norm in (17) is zero and inversion gives PI=0P_I=0; there is no omitted channel.

For negative time apply the same construction to −H-H and −P0-P_0, using W~(ξ,s)=W(ξ,−s)\widetilde W(\xi,s)=W(\xi,-s). Its positive-time wave is the original negative-time wave. The boundary solutions correspond through

R+−H(−λ)=−R−H(λ).(34) R_+^{-H}(-\lambda)=-R_-^H(\lambda). \tag{34}

The forcing changes to −f-f; any scalar sign in its stationary normalization is a unit phase. The range conclusion has no such ambiguity. This proves (3) for both signs.

Write Pac=EH(Ω)P_{\mathrm{ac}}=E_H(\Omega). Completeness gives W±W±∗=Pac\mathcal W_\pm\mathcal W_\pm^*=P_{\mathrm{ac}} and W±∗W±=1\mathcal W_\pm^*\mathcal W_\pm=1. Hence

S∗S=W−∗PacW−=1,SS∗=1.(35) \mathcal S^*\mathcal S =\mathcal W_-^*P_{\mathrm{ac}}\mathcal W_-=1, \qquad \mathcal S\mathcal S^*=1. \tag{35}

Wave group intertwining implies that S\mathcal S commutes with the free group. Its strong difference quotients then show preservation of D(H0)\mathcal D(H_0) and commutation with H0H_0 there. Spectral intertwining also gives commutation with every bounded Borel energy multiplier. Finally (4) follows by taking adjoints and using Plancherel. These transforms vanish on eigenvectors and are onto the full momentum space. Formula (31) identifies their band restrictions with the local-amplitude construction. Theorem 1.1 is proved. ∎

8. Changing a scalar modifier changes a unit phase

Theorem 8.1. Suppose another real scalar phase W′(ξ,t)W'(\xi,t) satisfies the phase, velocity and short-range cone hypotheses of Modified waves and the direction of escape, for this HH and one time sign. Let its modified wave be W′\mathcal W'. Then there is a measurable N(ξ)N(\xi), with ∣N∣=1|N|=1 almost everywhere, such that

W′=WN(D),(36) \mathcal W'=\mathcal W N(D), \tag{36}

where W\mathcal W is the complete wave of that sign. In particular W′\mathcal W' is complete.

Proof. Set At=eitHe−iW(D,t)A_t=e^{itH}e^{-iW(D,t)}, and define At′A'_t with W′W'. The wave existence and intertwining theorem puts the range of W′\mathcal W' in Hac(H)=ran⁡W\mathcal H_{\mathrm{ac}}(H)=\operatorname{ran}\mathcal W. For y=Why=\mathcal Wh, unitarity gives

∥At∗y−h∥=∥y−Ath∥⟶0.(37) \|A_t^*y-h\|=\|y-A_th\|\longrightarrow0. \tag{37}

Combine this convergence on the range with At′u→W′uA'_tu\to\mathcal W'u. The comparison thus converges strongly on every vector:

At∗At′⟶W∗W′,At∗At′=F−1ei(W−W′)F.(38) \begin{aligned} A_t^*A'_t&\longrightarrow\mathcal W^*\mathcal W',\\ A_t^*A'_t&=\mathcal F^{-1}e^{i(W-W')}\mathcal F. \end{aligned} \tag{38}

To identify this limit in momentum space, take increasing bounded boxes BkB_k covering Rn\mathbb R^n. Apply the strong limit to 1Bk1_{B_k}, defining an L2(Bk)L^2(B_k) function NkN_k. Every approximating multiplier commutes with frequency indicators; the limit does too. Therefore Nl=NkN_l=N_k on Bk⊂BlB_k\subset B_l. On each box, the summable-squared-error argument proved in Section 6 gives an almost-everywhere convergent subsequence along times tending to the selected infinity. It preserves the modulus one of the approximating phases. The countable union of the exceptional null sets is null, so the compatible functions define one measurable NN with ∣N∣=1|N|=1. Indicator tests inside each box give multiplication by NN; simple-function approximation and the uniform operator bound extend this to all L2L^2.

Consequently W∗W′=N(D)\mathcal W^*\mathcal W'=N(D). Since the range of W′\mathcal W' lies in the range of W\mathcal W, multiplication on the left by W\mathcal W proves (36). The multiplier is unitary and onto, so the two wave ranges coincide. ∎

This conclusion uses the exact scalar frequency multiplication in (38). Commutation with energy alone would permit mixing different frequencies of the same energy.

Use the conclusion

Construct a preimage on one good energy band, then account for all continuous states using the stated exceptional-energy set. Changing a scalar modifier changes a unit phase; it must not change the completeness claim.

9. Exercises with complete solutions

Exercise 1 — Basic: the two free channels. On the line take H0=D2H_0=D^2, λ=k2>0\lambda=k^2>0, and Schwartz forcing ff. Compute both outgoing amplitudes of R0,+(λ)fR_{0,+}(\lambda)f with the unitary Fourier convention. Express the spectral density in terms of those amplitudes and explain the negative spatial direction.

Solution 1. The upper-boundary Green function is

Kλ(x)=i2keik∣x∣,(−∂x2−k2)Kλ=δ0.(39) K_\lambda(x)=\frac{i}{2k}e^{ik|x|},\qquad (-\partial_x^2-k^2)K_\lambda=\delta_0. \tag{39}

The derivative jump is K′(0+)−K′(0−)=−1K'(0+)-K'(0-)=-1, which gives the delta after applying the negative second derivative. To select the boundary sign, take z=k2+iεz=k^2+i\varepsilon and its square root κ\kappa with positive imaginary part. The integrable decaying kernel ieiκ∣x∣/(2κ)i e^{i\kappa|x|}/(2\kappa) has the same derivative jump and solves (−∂x2−z)Kz=δ0(-\partial_x^2-z)K_z=\delta_0. Fourier transformation therefore gives its convolution multiplier (ξ2−z)−1(\xi^2-z)^{-1}, since this denominator has no real zeros. As ε↓0\varepsilon\downarrow0, κ→k\kappa\to k; bounded convergence against Schwartz tests gives (39) as exactly the upper boundary. Splitting its convolution at y=xy=x and letting the integrable forcing tails tend to zero gives

a+=lim⁡x→+∞e−ikx(Kλ∗f)(x)=i2π2kf^(k),a−=lim⁡x→−∞eikx(Kλ∗f)(x)=i2π2kf^(−k).(40) \begin{aligned} a_+&=\lim_{x\to+\infty}e^{-ikx}(K_\lambda*f)(x) =\frac{i\sqrt{2\pi}}{2k}\widehat f(k),\\ a_-&=\lim_{x\to-\infty}e^{ikx}(K_\lambda*f)(x) =\frac{i\sqrt{2\pi}}{2k}\widehat f(-k). \end{aligned} \tag{40}

For the negative spatial direction take s=−xs=-x and reflected momentum ξ′=−ξ\xi'=-\xi. The distinguished velocity becomes +2k+2k. Both outgoing amplitudes have the same +i+i factor. The shell consists of two points, with counting measure and g=2kg=2k, so

qf(λ)=∣f^(k)∣2+∣f^(−k)∣22k=kπ(∣a+∣2+∣a−∣2).(41) \begin{aligned} q_f(\lambda) &=\frac{|\widehat f(k)|^2+|\widehat f(-k)|^2}{2k}\\ &=\frac{k}{\pi}(|a_+|^2+|a_-|^2). \end{aligned} \tag{41}

This checks both the velocity factor and the unitary Fourier normalization.

Exercise 2 — Intermediate: assemble the channels. On a compact regular shell let ∑νχν=1\sum_\nu\chi_\nu=1 be a finite smooth partition. Suppose FjF_j are globally defined shell functions and each χνFj\chi_\nu F_j converges strongly in weighted shell L2L^2, uniformly over a compact energy interval under fixed chart trivializations. Prove existence and partition independence of the global limit. Explain why unrelated constants in the chart phases obstruct this argument.

Solution 2. The triangle inequality gives

∥Fj−Fl∥L2(dS/g)≤∑ν∥χν(Fj−Fl)∥L2(dS/g).(42) \begin{aligned} &\|F_j-F_l\|_{L^2(dS/g)}\\ &\quad\le\sum_\nu\|\chi_\nu(F_j-F_l)\|_{L^2(dS/g)}. \end{aligned} \tag{42}

The finite sum tends uniformly to zero. Completeness gives one global limit FF. Each bounded multiplier χν\chi_\nu then gives the local limit χνF\chi_\nu F, so every local channel relation holds for this function. Another partition approximates the same sequence FjF_j; uniqueness of its Hilbert-space limit proves independence. Adding a constant θν\theta_\nu to a chart phase multiplies its corrected amplitude by e−iθνe^{-i\theta_\nu}. Two different choices can assign different values to the same nonzero overlap. A single normalized global finite-range action ensures that all charts approximate one sequence.

Exercise 3 — Intermediate: a weak phase can lose all its norm. On L2([0,2π])L^2([0,2\pi]), let MjM_j be multiplication by eijξe^{ij\xi}. Prove weak-star convergence to zero in L∞L^\infty. Take Uj=1U_j=1, Jj=MjJ_j=M_j, and check (Uju,v)=(Mju,Jjv)(U_ju,v)=(M_ju,J_jv). Which convergence required in Section 6 fails?

Solution 3. Integration by parts against h∈C1([0,2π])h\in C^1([0,2\pi]) bounds the oscillatory integral by (∣h(0)∣+∣h(2π)∣+∥h′∥1)/j(|h(0)|+|h(2\pi)|+\|h'\|_1)/j. Approximate any L1L^1 test by C1C^1 tests. The remaining pairing is bounded by the L1L^1 approximation error since ∣eijξ∣=1|e^{ij\xi}|=1. Choose that approximation and then jj; this proves weak-star convergence to zero.

Every MjM_j is unitary, so (Mju,Mjv)=(u,v)(M_ju,M_jv)=(u,v), proving the proposed identity. But for v=1v=1, orthogonality of distinct integer exponentials gives

∥Jjv−Jlv∥22=4π,j≠l.(43) \|J_jv-J_lv\|_2^2=4\pi,\qquad j\ne l. \tag{43}

Thus the stationary maps do not converge strongly even on this vector. Strong convergence of JI(j)vJ_I^{(j)}v was essential to freeze its L1L^1 product before passing the weak-star phase limit. Without it the limit phase may be zero.

Exercise 4 — Advanced: quantitative norm rigidity. Let J:H→KJ:\mathcal H\to K satisfy J∗J=PJ^*J=P, where PP is an orthogonal projection. Take K=L2(X)K=L^2(X) with XX sigma-finite, and suppose U=J∗MU=J^*M, ∣M∣≤1|M|\le1. If ∥Uq∥≥(1−ϵ)∥q∥\|Uq\|\ge(1-\epsilon)\|q\| for all qq, with 0≤ϵ<10\le\epsilon<1, bound 1−∣M∣21-|M|^2 almost everywhere. For ϵ=0\epsilon=0, find a preimage of every v=Pvv=Pv.

Solution 4. Since ∥J∗∥≤1\|J^*\|\le1,

(1−ϵ)2∥q∥2≤∥Mq∥2=∫X∣M∣2∣q∣2.(44) (1-\epsilon)^2\|q\|^2 \le\|Mq\|^2=\int_X|M|^2|q|^2. \tag{44}

On a finite-measure subset where ∣M∣2<(1−ϵ)2|M|^2<(1-\epsilon)^2 by a fixed positive amount, the characteristic-function test contradicts (44). Use a sigma-finite exhaustion and a countable union over positive margins. The conclusion is 0≤1−∣M∣2≤2ϵ−ϵ20\le1-|M|^2\le2\epsilon-\epsilon^2 almost everywhere. At ϵ=0\epsilon=0 this gives ∣M∣=1|M|=1. Set q=M‾Jvq=\overline M Jv; then Uq=J∗MM‾Jv=Pv=vUq=J^*M\overline M Jv=Pv=v. Also J=JPJ=JP, so the range of UU lies in PHP\mathcal H and is exactly that subspace. In the Fourier identification of the free space this is the preimage in (30).

Exercise 5 — Advanced: energy commutation is weaker. In momentum L2(R)L^2(\mathbb R), let P0(ξ)=ξ2P_0(\xi)=\xi^2 and Rq(ξ)=q(−ξ)Rq(\xi)=q(-\xi). Show that RR is unitary and commutes with every bounded Borel function of P0P_0, but cannot be multiplication by a scalar phase. Explain what extra identity for two scalar time modifiers rules out this phenomenon.

Solution 5. Reflection preserves Lebesgue measure, and R2=1R^2=1, so RR is unitary. Since P0(−ξ)=P0(ξ)P_0(-\xi)=P_0(\xi), it commutes with every b(P0)b(P_0). A nonzero function supported in (1,2)(1,2) is sent to one supported in (−2,−1)(-2,-1). A scalar multiplier preserves the original support, so it cannot equal RR.

For two scalar modifiers their comparison has the exact identity

At∗At′=F−1ei(W−W′)F.(45) A_t^*A'_t=\mathcal F^{-1}e^{i(W-W')}\mathcal F. \tag{45}

It commutes with every frequency indicator, including indicators separating equal-energy channels. On the complete wave range the adjoints converge strongly, as in (37), giving a strong limit of (45). Indicator tests on increasing bounded boxes construct compatible local L2L^2 functions NN, and almost-everywhere subsequences preserve ∣N∣=1|N|=1. Simple-function approximation identifies the full limit with multiplication by NN. Thus modifier ambiguity is a scalar frequency phase, whereas the scattering operator can mix equal-energy channels.

References