Asymptotic completeness for short-range operators

Written by GPT-6.1 Sol (OpenAI) and GPT-6 Astra (OpenAI). Original exposition: CC0.

Working question: How does a time comparison prove that no continuous states are missing? A wave operator can preserve every norm and still miss a subspace. The unilateral shift in the guide makes this visible. Here the matching-sign composition with a stationary transform equals the ordinary Fourier transform. Its surjectivity is the extra information that recovers every continuous interacting state.

The time-dependent wave operators and the stationary distorted Fourier transforms describe the same continuous states. Their composition is the ordinary Fourier transform. Because that transform is onto, every absolutely continuous perturbed state has both an incoming and an outgoing free comparison state.

Use the real simply characteristic polynomial pp, its absence of invariant directions, the symmetric short-range differential perturbation VV, and the self-adjoint closure HH from Wave operators for differential perturbations. Write H0=p(D)H_0=p(D), and use the unitary Fourier transform F\mathcal F. The existence theorem there gives isometries

W±=s ⁣− ⁣limt→±∞eitHe−itH0.(1) W_\pm=\mathop{\mathrm{s\!-\!lim}}_{t\to\pm\infty} e^{itH}e^{-itH_0}. \tag{1}

Distorted Fourier transforms and spectral density supplies J±J_\pm, the closed countable exceptional set Σ\Sigma, its complement Ω\Omega, and the projection Ec=EH(Ω)E^c=E_H(\Omega). In particular,

∥J±u∥2=∥Ecu∥2,J±eitH=eitMpJ±.(2) \|J_\pm u\|_2=\|E^cu\|_2,\qquad J_\pm e^{itH}=e^{itM_p}J_\pm. \tag{2}

The same lesson proves Hac(H)=EcL2\mathcal H_{\mathrm{ac}}(H)=E^cL^2, and the existence theorem puts the ranges of W±W_\pm inside this subspace.

For further reading on stationary spectral representations and scattering completeness, see Kuroda [K], Section 4.2, Yafaev [Y], Section 2, and Teschl [T], Section 12.1.

1. Damped integrals and their two signs

The continuous Banach-valued integrals below use the norm-integral construction and continuous primitive theorem from Hilbert-valued integration, whose proofs also apply to arbitrary Banach spaces. Completeness and the scalar norm bound construct the improper integrals. Bounded linear maps commute with them, first on Riemann sums and then by the norm limit. In Section 2 we prove the additional interchange with surface representatives directly from scalar Fubini.

Let D=F−1Cc∞({∇p≠0}),Ft=e−itH0f,f∈D. \mathcal D=\mathcal F^{-1}C_c^\infty(\{\nabla p\ne0\}), \qquad F_t=e^{-itH_0}f,\quad f\in\mathcal D. The wave-packet and shell-integrability proof shows density of D\mathcal D and ∫R∥VFt∥2 dt<∞.(3) \int_{\mathbb R}\|VF_t\|_2\,dt<\infty. \tag{3} Its product derivative therefore gives W+f=f+∫0∞ieitHVFt dt,W−f=f−∫−∞0ieitHVFt dt,(4) W_+f=f+\int_0^\infty i e^{itH}VF_t\,dt,\qquad W_-f=f-\int_{-\infty}^0 i e^{itH}VF_t\,dt, \tag{4} with absolutely convergent L2L^2 integrals.

Lemma 1.1. The function t↦VFtt\mapsto VF_t is continuous and bounded in BB. For ε>0\varepsilon>0, λ∈R\lambda\in\mathbb R, and σ∈{+1,−1}\sigma\in\{+1,-1\}, σ∫σt>0ie−ε∣t∣eitλVFt dt=VR0(λ+σiε)fin B.(5) \sigma\int_{\sigma t>0} i e^{-\varepsilon|t|}e^{it\lambda}VF_t\,dt =VR_0(\lambda+\sigma i\varepsilon)f \quad\text{in }B. \tag{5}

Proof. All graph components of FtF_t have their free L2L^2 norms preserved, so ∥Ft∥Xp≤∑α∥(∂αp)(D)f∥2(t∈R).(6) \|F_t\|_{X_p} \leq\sum_\alpha\|(\partial^\alpha p)(D)f\|_2 \quad(t\in\mathbb R). \tag{6} Each component is L2L^2-continuous in tt, by dominated convergence of its Fourier phase. Since the B∗B^* norm is bounded by the L2L^2 norm, the path is continuous in XpX_p. Boundedness of V:Xp→BV:X_p\to B proves the first claim. The exponential damping makes (5) absolutely convergent in BB, and also makes its free input integral absolutely convergent in XpX_p.

For a real scalar aa, i∫0∞e−εte−ita dt=1a−iε,−i∫−∞0eεte−ita dt=1a+iε.(7) i\int_0^\infty e^{-\varepsilon t}e^{-ita}\,dt =\frac1{a-i\varepsilon},\qquad -i\int_{-\infty}^0e^{\varepsilon t}e^{-ita}\,dt =\frac1{a+i\varepsilon}. \tag{7} Apply these identities with a=p(ξ)−λa=p(\xi)-\lambda. Each free graph component has a fixed compact smooth Fourier amplitude. On a finite time interval, the bounded Fourier map commutes with the norm integral; scalar integration gives the truncated version of (7). Its remaining scalar tail is bounded by e−εT/εe^{-\varepsilon T}/\varepsilon, uniformly in the real number aa. Multiplying by each fixed L2L^2 Fourier amplitude therefore bounds its tail norm by e−εT/εe^{-\varepsilon T}/\varepsilon times that amplitude norm. Passing to infinity in all finitely many graph components identifies the free input integral with R0(λ+σiε)fR_0(\lambda+\sigma i\varepsilon)f. Applying the bounded map VV to the XpX_p integral proves (5). □\square

The undamped integral in (4) is controlled in L2L^2 by (3). Formula (5) uses a separate BB integral with damping; no undamped time integrability in BB is required.

2. Comparing time evolution with the surface transform

For λ∈Ω\lambda\in\Omega let Aσ(λ)=(I+VR0,σ(λ))−1:B→B. A_\sigma(\lambda)=(I+VR_{0,\sigma}(\lambda))^{-1}:B\to B. The boundary-family proof proves its strong continuity, local uniform norm bounds, and strong continuity of VR0(z)VR_0(z) up to each boundary.

Theorem 2.1. With matching signs, J±W±=Fon L2(dx).(8) J_\pm W_\pm=\mathcal F \quad\text{on }L^2(dx). \tag{8}

Proof. Start with f∈Df\in\mathcal D. For ε>0\varepsilon>0, set yσ,ε=f+σ∫σt>0ie−ε∣t∣eitHVFt dt.(9) y_{\sigma,\varepsilon} =f+\sigma\int_{\sigma t>0} i e^{-\varepsilon|t|}e^{itH}VF_t\,dt. \tag{9} Dominated convergence using (3) gives yσ,ε→Wσfy_{\sigma,\varepsilon}\to W_\sigma f in L2L^2. Boundedness and (2) give Jσyσ,ε=Jσf+σ∫σt>0ie−ε∣t∣eitMpJσ(VFt) dt⟶JσWσfin L2(dξ).(10) J_\sigma y_{\sigma,\varepsilon} =J_\sigma f+\sigma\int_{\sigma t>0} i e^{-\varepsilon|t|}e^{itM_p}J_\sigma(VF_t)\,dt \longrightarrow J_\sigma W_\sigma f \quad\text{in }L^2(d\xi). \tag{10}

We spell out how to interpret this time integral on surfaces. The path b(t)=VFtb(t)=VF_t is continuous in BB. On every compact (λ,t)(\lambda,t) set in Ω×R\Omega\times\mathbb R, Aσ(λ)b(t)A_\sigma(\lambda)b(t) is continuous in BB: split the difference into the change in bb, controlled by the local uniform norm bound, and the change in AσA_\sigma on a fixed vector. The parameter partition and measurable-assembly proof therefore applies with tt as an additional parameter. Approximate this BB-valued function by locally finite smooth partitions of unity in (λ,t)(\lambda,t), with fixed compact-Fourier values. More explicitly, let hj(λ,t)h_j(\lambda,t) be these approximations, with BB-error at most 2−j2^{-j}, and form Gj(t,ξ)=Fhj(p(ξ),t)(ξ)G_j(t,\xi)=\mathcal Fh_j(p(\xi),t)(\xi). Each is locally a finite sum of continuous functions, hence jointly Borel. At every fixed (λ,t)(\lambda,t) the trace errors are summable in surface L2L^2, so the sequence converges outside a surface-null set to TλAσ(λ)b(t)T_\lambda A_\sigma(\lambda)b(t). The pointwise Cauchy set in (t,ξ)(t,\xi) is Borel; define the limit there and zero elsewhere. Coarea at each fixed tt identifies this function with the already defined L2L^2 class Jσb(t)J_\sigma b(t). This constructs the representatives needed for Fubini, rather than choosing arbitrary ambient L2L^2 values.

On a compact energy interval I⋐ΩI\Subset\Omega, the trace and inverse bounds and Lemma 1.1 give ∥TλAσ(λ)b(t)∥L2(dS)≤CI,f(λ∈I, t∈R).(11) \|T_\lambda A_\sigma(\lambda)b(t)\|_{L^2(dS)} \leq C_{I,f} \quad(\lambda\in I,\ t\in\mathbb R). \tag{11} With the factor e−ε∣t∣e^{-\varepsilon|t|}, this is integrable in tt. Here is the required interchange proof. On a compact frequency patch KK inside one energy chart, g−1g^{-1} is bounded; coarea and (11) bound the L2(K)L^2(K) norm of the jointly measurable integrand by CKe−ε∣t∣C_K e^{-\varepsilon|t|}. More generally, for jointly measurable F(t,ξ)F(t,\xi) on R×K\mathbb R\times K with M=∫R∥F(t,⋅)∥L2(K) dt<∞, M=\int_{\mathbb R}\|F(t,\cdot)\|_{L^2(K)}\,dt<\infty, Tonelli and Cauchy–Schwarz give ∫ ⁣∫K∣F∣≤∣K∣1/2M\int\!\int_K|F|\leq |K|^{1/2}M. The scalar integral h(ξ)=∫F(t,ξ) dth(\xi)=\int F(t,\xi)\,dt therefore exists almost everywhere. For q∈L2(K)q\in L^2(K), the integral of ∣Fq‾∣|F\overline q| is at most M∥q∥2M\|q\|_2, so scalar Fubini gives (h,q)=∫(F(t),q) dt(h,q)=\int(F(t),q)\,dt. To verify h∈L2h\in L^2 without assuming it, test with q=h1{∣h∣≤N}q=h\mathbf1_{\{|h|\leq N\}}, which lies in L2(K)L^2(K) since KK has finite measure. The resulting inequality bounds ∥h1{∣h∣≤N}∥2\|h\mathbf1_{\{|h|\leq N\}}\|_2 by MM. Monotone convergence gives ∥h∥2≤M\|h\|_2\leq M. Bounded scalar pairings commute with the continuous vector integrals already constructed, so equality of all these pairings identifies their L2(K)L^2(K) integral with hh.

The same argument applies on each compact surface patch with dSdS, for each fixed energy: the canonical trace is continuous in tt and its norm has the integrable bound (11) with damping. Scalar Fubini in (t,λ,η)(t,\lambda,\eta) on each coordinate patch then identifies these surface integrals with the ambient representative for almost every energy. A countable patch cover suffices. Thus (10) is identified, for almost every energy and surface point, with the measurable surface expression Gσ,ε∣Mλ=TλAσ(λ)[f+VR0(λ+σiε)f].(12) G_{\sigma,\varepsilon}|_{M_\lambda} =T_\lambda A_\sigma(\lambda) [f+VR_0(\lambda+\sigma i\varepsilon)f]. \tag{12} Indeed eitMpe^{itM_p} becomes the scalar eitλe^{it\lambda} on that surface, and (5) evaluates its remaining BB integral. For the identification in ambient L2L^2, the integral in (10) is absolutely convergent there by (3); the locally defined surface integrals give the same representative by Fubini on a countable energy-coordinate cover. This requires only equality at almost every energy for the time integral.

For every fixed λ∈Ω\lambda\in\Omega, strong boundary continuity gives VR0(λ+σiε)f⟶VR0,σ(λ)fin B. VR_0(\lambda+\sigma i\varepsilon)f \longrightarrow VR_{0,\sigma}(\lambda)f\quad\text{in }B. Thus (12) tends in surface L2L^2 to TλAσ(λ)(I+VR0,σ(λ))f=Tλf.(13) T_\lambda A_\sigma(\lambda) (I+VR_{0,\sigma}(\lambda))f =T_\lambda f. \tag{13} This convergence also holds in L2L^2 on every compact frequency subset of p−1(Ω)p^{-1}(\Omega). To see it, its image under pp lies in a compact subset of Ω\Omega; cover that energy set by finitely many compact intervals there. All free graph, inverse and trace norms are uniformly bounded on this compact set, including 0≤ε≤ε00\leq\varepsilon\leq\varepsilon_0. Surface squared differences in (13) are therefore uniformly bounded and tend to zero. On the compact frequency set, g=∣∇p∣g=|\nabla p| has a positive minimum, since its energies lie in Ω\Omega. Thus the coarea factor 1/g1/g is uniformly bounded on that set. Integrating the surface squared differences over the finite energy cover and applying dominated convergence gives the claimed local L2L^2 convergence.

The global L2L^2 limit in (10) and this local limit must agree. Since ff has smooth Fourier support, TλfT_\lambda f is the restriction of f^\widehat f. A countable compact exhaustion of p−1(Ω)p^{-1}(\Omega) proves JσWσf=f^J_\sigma W_\sigma f=\widehat f there. Its complement p−1(Σ)p^{-1}(\Sigma) is null, as proved in the distorted-transform lesson, so (8) holds in full L2(dξ)L^2(d\xi) on D\mathcal D. Density of D\mathcal D, boundedness of JσJ_\sigma, isometry of WσW_\sigma, and unitary Plancherel extend it to every ff. □\square

3. Completeness and the scattering operator

Theorem 3.1. The maps W±:L2(dx)⟶EcL2(dx),J±:EcL2(dx)⟶L2(dξ)(14) W_\pm:L^2(dx)\longrightarrow E^cL^2(dx),\qquad J_\pm:E^cL^2(dx)\longrightarrow L^2(d\xi) \tag{14} are unitary onto the indicated spaces. In particular ran⁡W+=ran⁡W−=Hac(H).(15) \operatorname{ran}W_+=\operatorname{ran}W_- =\mathcal H_{\mathrm{ac}}(H). \tag{15} The scattering operator S=W+∗W−(16) S=W_+^*W_- \tag{16} is unitary on the free space and commutes with eitH0e^{itH_0}. In momentum space, FSF−1=J+J−−1,(17) \mathcal F S\mathcal F^{-1} =J_+J_-^{-1}, \tag{17} where the inverse in (17) is the inverse of J−J_- restricted to EcL2E^cL^2.

Proof. WσW_\sigma is already an isometry with range in EcL2E^cL^2, and JσJ_\sigma is an isometry on that subspace. Equation (8) and surjectivity of F\mathcal F first prove that JσJ_\sigma is onto. For u∈EcL2u\in E^cL^2, choose f=F−1Jσuf=\mathcal F^{-1}J_\sigma u. Then JσWσf=Ff=JσuJ_\sigma W_\sigma f=\mathcal Ff=J_\sigma u. The difference Wσf−uW_\sigma f-u lies in EcL2E^cL^2, where JσJ_\sigma is injective, so it is zero. This proves surjectivity of WσW_\sigma and (14)-(15).

An isometry onto EcL2E^cL^2 satisfies Wσ∗Wσ=IW_\sigma^*W_\sigma=I and WσWσ∗=EcW_\sigma W_\sigma^*=E^c: the latter operator is the identity on the range and zero on its orthogonal complement. Consequently S∗S=W−∗EcW−=IS^*S=W_-^*E^cW_-=I, and similarly SS∗=ISS^*=I. The group intertwining and its adjoint give SeitH0=W+∗eitHW−=eitH0SSe^{itH_0}=W_+^*e^{itH}W_-=e^{itH_0}S.

Equation (8) on the common range gives FW+∗=J+\mathcal F W_+^*=J_+, while W−F−1=J−−1W_-\mathcal F^{-1}=J_-^{-1}. Their composition proves (17). □\square

The spectral-measure argument in Modified waves and the direction of escape applies to the isometry SS intertwining the free group with itself. It proves ∥E0(A)Sf∥2=∥E0(A)f∥2\|E_0(A)Sf\|^2=\|E_0(A)f\|^2 for every vector and every Borel energy set AA, by the damped resolvent integral and scalar spectral inversion. Polarization gives S∗E0(A)S=E0(A)S^*E_0(A)S=E_0(A); multiplication on the left by the now proved unitary SS gives SE0(A)=E0(A)SSE_0(A)=E_0(A)S. In momentum space these projections multiply by 1{p(ξ)∈A}\mathbf1_{\{p(\xi)\in A\}}. Thus (17) restricts to a unitary on every such energy region. The operator on an individual energy surface requires the further stationary scattering-matrix construction.

The closed-operator domain identities are included in this unitary equivalence. The earlier inclusion HWσf=WσH0fHW_\sigma f=W_\sigma H_0f for f∈D(H0)f\in\mathcal D(H_0), together with the unitary group equivalence and its generator domains, gives WσD(H0)=D(H)∩EcL2. W_\sigma\mathcal D(H_0)= \mathcal D(H)\cap E^cL^2. The orthogonal complement is the closed span of bound states, including any threshold eigenfunctions. This completeness theorem does not impose decay or finite multiplicity at thresholds.

Example 3.2. A bounded real potential satisfying ∣V(x)∣≤C(1+∣x∣)[log⁡(e+∣x∣)]2 |V(x)|\leq \frac{C}{(1+|x|)[\log(e+|x|)]^2} is covered by the summable local criterion and logarithmic example and hence by (15). For H0=−ΔH_0=-\Delta, the derivative weight satisfies p~(ξ)2=∣ξ∣4+4∣ξ∣2+4n≤Cn(1+∣ξ∣2)2\widetilde p(\xi)^2=|\xi|^4+4|\xi|^2+4n\leq C_n(1+|\xi|^2)^2, which proves the simply characteristic inequality p~≤C(1+∣p∣+∣∇p∣)\widetilde p\leq C(1+|p|+|\nabla p|). If p(ξ+tv)=p(ξ)p(\xi+tv)=p(\xi) for all tt, the quadratic coefficient ∣v∣2|v|^2 is zero, so there is no nonzero invariant direction. The cited logarithmic example proves that the envelope is slower than every fixed (1+∣x∣)−1−δ(1+|x|)^{-1-\delta}, while its dyadic contributions sum like ∑j(1+j)−2\sum_j(1+j)^{-2}. Completeness follows from the full local short-range condition and the stationary comparison, in addition to wave-operator existence.

The sign in the eigenfunction equation. Let H=H0+VH=H_0+V, R0(z)=(H0−z)−1R_0(z)=(H_0-z)^{-1}, and (H0−λ)ψ0=0(H_0-\lambda)\psi_0=0. With these conventions the outgoing integral equation is

ψ=ψ0−R0(λ+i0)Vψ. \psi=\psi_0-R_0(\lambda+i0)V\psi.

Indeed, wherever the boundary product is defined, applying H0−λH_0-\lambda gives (H0−λ)ψ=−Vψ(H_0-\lambda)\psi=-V\psi, as required by (H−λ)ψ=0(H-\lambda)\psi=0. The opposite sign would instead give (H0−λ)ψ=Vψ(H_0-\lambda)\psi=V\psi. Rearranging the correct equation and multiplying by VV gives (I+VR0,+)Vψ=Vψ0(I+VR_{0,+})V\psi=V\psi_0, explaining the plus inside the forcing inverse. Taking adjoints exchanges upper and lower resolvent boundaries; it does not change the sign of VV in HH. For eigenfunction expansions, see Yafaev [Y], Section 2.

A concrete verification of the sign. On the line take H0=−∂x2H_0=-\partial_x^2, λ=1\lambda=1, ψ0=eix\psi_0=e^{ix}, and

V=18w,w(x)={e−1/(1−x2),∣x∣<1,0,∣x∣≥1. V=\tfrac18w,\qquad w(x)=\begin{cases} e^{-1/(1-x^2)},&|x|<1,\\ 0,&|x|\geq1. \end{cases}

The smooth cutoff construction makes ww smooth across its endpoints. This real smooth compact potential satisfies the local short-range criterion, and the bounded-perturbation domain proof makes H=H0+VH=H_0+V self-adjoint on H2(R)H^2(\mathbb R). The free upper boundary kernel is G(x)=(i/2)ei∣x∣G(x)=(i/2)e^{i|x|}: it solves −G′′−G=0-G''-G=0 off zero and has derivative jump −1-1. Integrating by parts on the two half-lines against a compactly supported smooth test leaves minus that jump times its value at zero; the continuity of GG cancels the terms containing the derivative of the test. Hence −G′′−G=δ0-G''-G=\delta_0.

To identify it with the resolvent boundary, put z=1+iεz=1+i\varepsilon, aε=((1+ε2+1)/2)1/2a_\varepsilon=((\sqrt{1+\varepsilon^2}+1)/2)^{1/2}, bε=ε/(2aε)b_\varepsilon=\varepsilon/(2a_\varepsilon), and κε=aε+ibε\kappa_\varepsilon=a_\varepsilon+ib_\varepsilon. Then κε2=z\kappa_\varepsilon^2=z, bε>0b_\varepsilon>0, and κε→1\kappa_\varepsilon\to1. The kernel Gε(x)=ieiκε∣x∣/(2κε)G_\varepsilon(x)=i e^{i\kappa_\varepsilon|x|}/(2\kappa_\varepsilon) is in L1∩L2L^1\cap L^2, and the same derivative-jump computation gives (−∂x2−z)Gε=δ0( -\partial_x^2-z)G_\varepsilon=\delta_0. For compactly supported bounded hh, which belongs to BB because it meets only finitely many dyadic shells, Young's inequality puts v=Gε∗hv=G_\varepsilon*h in L2L^2. Distributional differentiation gives v′′=−zv−h∈L2v''=-zv-h\in L^2; Plancherel then gives ξ2v^∈L2\xi^2\widehat v\in L^2, hence v∈H2v\in H^2. Uniqueness of the nonreal self-adjoint resolvent solution proves v=R0(z)hv=R_0(z)h. The kernels converge uniformly on compact sets to GG, so convolution with this compactly supported L1L^1 function converges locally uniformly to G∗hG*h. The free boundary limit also converges as a distribution, by the earlier limiting-absorption theorem. Uniqueness of that limit proves R0,+(1)h=G∗hR_{0,+}(1)h=G*h.

On I=[−1,1]I=[-1,1], let K:C(I)→C(I)K:C(I)\to C(I) be

(Kh)(x)=i16∫Iei∣x−y∣w(y)h(y) dy. (Kh)(x)=\frac{i}{16}\int_I e^{i|x-y|}w(y)h(y)\,dy.

The uniform limit of continuous functions is continuous, and a uniformly Cauchy sequence has a pointwise limit by scalar completeness; thus C(I)C(I) is complete. Since 0≤w≤10\leq w\leq1, the integral gives ∥K∥≤1/8\|K\|\leq1/8. It also gives ∣Kh(x)−Kh(x′)∣≤∥h∥∞∣x−x′∣/8|Kh(x)-Kh(x')|\leq\|h\|_\infty|x-x'|/8, using ∣eiu−eiv∣≤∣u−v∣|e^{iu}-e^{iv}|\leq|u-v|, which follows by integrating the derivative of the exponential. Thus KK indeed maps C(I)C(I) to itself. The Neumann inverse (I+K)−1=∑m≥0(−K)m(I+K)^{-1}=\sum_{m\geq0}(-K)^m therefore converges in norm, with its tail bounded by (1/8)N+1/(1−1/8)(1/8)^{N+1}/(1-1/8). The finite partial sums satisfy (I+K)∑m=0N(−K)m=I−(−K)N+1(I+K)\sum_{m=0}^N(-K)^m=I-(-K)^{N+1}, and the same identity holds in the other order. The remainder norm tends to zero, proving both inverse identities. Put ψI=(I+K)−1ψ0∣I\psi_I=(I+K)^{-1}\psi_0|_I. Then

∥ψI−ψ0∥∞≤17,∣ψI∣≥67on I. \begin{gathered} \|\psi_I-\psi_0\|_\infty\leq\tfrac17,\\ |\psi_I|\geq\tfrac67\quad\text{on }I. \end{gathered}

Extend it to the line by

ψ(x)=eix−i16∫Iei∣x−y∣w(y)ψI(y) dy. \psi(x)=e^{ix}-\frac{i}{16}\int_I e^{i|x-y|}w(y)\psi_I(y)\,dy.

The defining equation on II proves that this extension restricts to ψI\psi_I. The kernel identity gives (H−1)ψ=0(H-1)\psi=0 distributionally. Here are the regularity details. The integral makes ψ\psi continuous, so F=(V−1)ψF=(V-1)\psi is continuous and ψ′′=F\psi''=F distributionally. On any bounded open interval, twice integrating FF from an interior point gives a C2C^2 function PP with P′′=FP''=F. A distribution with zero first derivative is constant: every compactly supported smooth test of integral zero has a compactly supported smooth primitive, so the distribution annihilates it; subtracting a fixed test of integral one identifies its value on every test. Applying this fact first to (ψ−P)′(\psi-P)' and then after subtracting the resulting linear function shows that ψ−P\psi-P is affine. Thus ψ\psi is C2C^2. The equation ψ′′=(V−1)ψ\psi''=(V-1)\psi and the scalar primitive theorem now raise its regularity by two derivatives at each step, giving ψ∈C∞\psi\in C^\infty. For x>1x>1, the correction is −ieix∫Ie−iyw(y)ψI(y) dy/16-i e^{ix}\int_Ie^{-iy}w(y)\psi_I(y)\,dy/16; for x<−1x<-1, it is −ie−ix∫Ieiyw(y)ψI(y) dy/16-i e^{-ix}\int_Ie^{iy}w(y)\psi_I(y)\,dy/16. These are exactly outgoing waves on their respective ends. Since ∣Vψ∣≥3w/28|V\psi|\geq3w/28 in (−1,1)(-1,1), it is nonzero. The residual of the opposite-sign equation is −2R0,+(1)Vψ-2R_{0,+}(1)V\psi; it cannot vanish, because applying −∂x2−1-\partial_x^2-1 would give −2Vψ=0-2V\psi=0. This nonzero smooth compact potential therefore rules out accidental cancellation in the opposite-sign equation.

Use the conclusion

Locate the matching signs in the Abel comparison, then write the preimage of a continuous state. Keep the stationary identity and the time-dependent existence theorem as distinct inputs to the range argument.

4. Exercises

Exercise 4.1 (foundation). Evaluate both scalar integrals in (7), including their signs, and determine the corresponding upper or lower resolvent parameter.

Exercise 4.2 (foundation). Let W:X→YW:X\to Y and J:Y→ZJ:Y\to Z be isometries of Hilbert spaces. If JW:X→ZJW:X\to Z is onto, prove that both JJ and WW are onto.

Exercise 4.3 (intermediate). Suppose the known estimate is ∫∥VFt∥2 dt<∞\int\|VF_t\|_2\,dt<\infty and sup⁡t∥VFt∥B<∞\sup_t\|VF_t\|_B<\infty. Identify which estimate justifies (10), and which justifies (5). Prove convergence of yσ,εy_{\sigma,\varepsilon} to WσfW_\sigma f without assuming ∫∥VFt∥B dt<∞\int\|VF_t\|_B\,dt<\infty.

Exercise 4.4 (intermediate). Derive (17) from the two identities J±W±=FJ_\pm W_\pm=\mathcal F and their unitary ranges. Specify the domain of each inverse and adjoint.

Exercise 4.5 (advanced). In the general theorem, prove the equality of the closed operator domains under WσW_\sigma from the group identity and surjectivity. Explain why the equality does not identify D(H)\mathcal D(H) with the full free domain as sets of functions.

5. Complete solutions

Solution 4.1. The positive-time integral is i/(ε+ia)=1/(a−iε)i/(\varepsilon+ia)=1/(a-i\varepsilon), since ε+ia=i(a−iε)\varepsilon+ia=i(a-i\varepsilon). The negative-time integral is −i/(ε−ia)=1/(a+iε)-i/(\varepsilon-ia)=1/(a+i\varepsilon), since ε−ia=−i(a+iε)\varepsilon-ia=-i(a+i\varepsilon). With a=p(ξ)−λa=p(\xi)-\lambda, they give R0(λ+iε)R_0(\lambda+i\varepsilon) and R0(λ−iε)R_0(\lambda-i\varepsilon), respectively. The minus sign in the negative-time version is part of (4); keeping it gives the plus VR0VR_0 correction on both sides in (12).

Solution 4.2. Surjectivity of JWJW immediately implies surjectivity of JJ. For y∈Yy\in Y, choose x∈Xx\in X with JWx=JyJWx=Jy. Injectivity of the isometry JJ gives Wx=yWx=y, proving surjectivity of WW. With the same proof, YY may be a specified closed subspace of a larger Hilbert space; only that subspace is the domain on which JJ must be isometric.

Solution 4.3. In (10), ∥JσeitHVFt∥2≤∥VFt∥2\|J_\sigma e^{itH}VF_t\|_2\leq\|VF_t\|_2, by boundedness of JσJ_\sigma and unitarity. This supplies the integrable L2L^2 majorant. In (5), the exponential factor and the uniform BB bound give ∫σt>0e−ε∣t∣∥VFt∥B dt≤C/ε\int_{\sigma t>0}e^{-\varepsilon|t|}\|VF_t\|_B\,dt\leq C/\varepsilon. The undamped BB integral is not used. Subtract (4) from (9) and estimate ∥yσ,ε−Wσf∥2≤∫σt>0∣e−ε∣t∣−1∣ ∥VFt∥2 dt. \|y_{\sigma,\varepsilon}-W_\sigma f\|_2 \leq\int_{\sigma t>0} |e^{-\varepsilon|t|}-1|\,\|VF_t\|_2\,dt. Its integrand tends pointwise to zero and is bounded by the integrable function ∥VFt∥2\|VF_t\|_2. Dominated convergence proves the limit.

Solution 4.4. The maps W±W_\pm are unitaries from the free L2(dx)L^2(dx) onto EcL2(dx)E^cL^2(dx); their adjoints restricted to this range are their inverse unitaries. The restrictions J±:EcL2(dx)→L2(dξ)J_\pm:E^cL^2(dx)\to L^2(d\xi) are unitaries. For u∈EcL2u\in E^cL^2, write u=W+fu=W_+f. Then J+u=Ff=FW+∗uJ_+u=\mathcal Ff=\mathcal F W_+^*u, proving FW+∗=J+\mathcal F W_+^*=J_+ on the range. Similarly J−W−F−1=IJ_-W_-\mathcal F^{-1}=I gives W−F−1=J−−1W_-\mathcal F^{-1}=J_-^{-1}, with inverse domain L2(dξ)L^2(d\xi) and target EcL2E^cL^2. Composing these identities with S=W+∗W−S=W_+^*W_- yields (17).

Solution 4.5. The group identity is eitHWσ=WσeitH0e^{itH}W_\sigma=W_\sigma e^{itH_0}. If f∈D(H0)f\in\mathcal D(H_0), differentiation at zero gives Wσf∈D(H)W_\sigma f\in\mathcal D(H) and HWσf=WσH0fHW_\sigma f=W_\sigma H_0f. Conversely, for u∈D(H)∩EcL2u\in\mathcal D(H)\cap E^cL^2, surjectivity supplies f=Wσ−1uf=W_\sigma^{-1}u. Applying that inverse to the group identity shows that the orbit eitH0fe^{itH_0}f is norm differentiable at zero. The self-adjoint generator-domain criterion gives f∈D(H0)f\in\mathcal D(H_0). Thus the domain equality is carried by the unitary WσW_\sigma. It compares a free function with its transformed perturbed state; it does not say the same function lies in both domains. Bound states lie outside this comparison subspace as well.

References