Short-time reduction of the curved Dirichlet remainder

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

This reading proves the uniform curved Dirichlet spectral remainder in the full scalar scope below. Sections 1–4 give positive unsmoothing and the exact cosine formula. Sections 5–30 retain detailed near-normal and complementary frozen-model arguments. Sections 31–38 give a complete second construction: a finite reflected wave expansion with its actual smooth error, coarse temporal Fourier bounds, and the uniform no-return kernel estimate. Together they prove (B16) and both bounds in (B138), including the wall and the interior.

The operator has the full scope used in Generalized rays and the Dirichlet Weyl law: a scalar formally self-adjoint second-order elliptic differential operator on half densities on a compact smooth manifold of dimension n≥2n\geq2, with smooth boundary, no corners, and strictly positive Dirichlet realization. All smooth lower-order terms are retained. Its principal symbol defines the metric gg; d=d(x)d=d(x) is inward metric distance in a fixed collar. Every diagonal density below is relative to dVgdV_g.

Read Smooth Dirichlet regularity, power domains, and projector growth, Sections 4–6, first. It proves the exact spectral realization, smooth eigenfunctions, and the uniform diagonal bound used here. The positive-measure argument develops the cumulative version of Return times and spectral counting, Lemma 1.1. Section 5 uses the already proved parameter Morse lemma and stationary phase with parameter remainders, equations (P1)–(P10). None of these inputs requires the curved estimate being reduced.

1. The positive measure and the reflected model

Write the orthonormal eigensections as uj(dVg)1/2u_j(dV_g)^{1/2}, with eigenvalues λj>0\lambda_j>0, and put κj=λj\kappa_j=\sqrt{\lambda_j}. At each point define μx=∑j∣uj(x)∣2δκj,Ex(k)=μx([0,k])(k≥0),Ex(k)=0(k<0),0≤Ex(k)≤C(1+k)n(k≥0).(B1) \begin{gathered} \mu_x=\sum_j|u_j(x)|^2\delta_{\kappa_j},\\ E_x(k)=\mu_x([0,k])\quad(k\geq0),\\ E_x(k)=0\quad(k<0),\\ 0\leq E_x(k)\leq C(1+k)^n\quad(k\geq0). \end{gathered} \tag{B1} The last bound is the cited programme proof, equation (26), with spectral parameter k2k^2; the bounded interval 0≤k≤10\leq k\leq1 is absorbed using monotonicity. Its constant is independent of xx, including the wall. One may instead use [0,k)[0,k) throughout.

The model cumulative function, extended by zero to negative arguments, is Md(k)=(2π)−n∫∣ξ∣≤k[1−cos⁡(2dξn)] dξ,k≥0,Md(k)=kn[Wn(0)−Wn(2kd)],Wn(s)=(2π)−n∫∣η∣≤1cos⁡(sηn) dη.(B2) \begin{gathered} M_d(k)=(2\pi)^{-n}\int_{|\xi|\leq k} [1-\cos(2d\xi_n)]\,d\xi,\\ k\geq0,\\ M_d(k)=k^n[W_n(0)-W_n(2kd)],\\ W_n(s)=(2\pi)^{-n}\int_{|\eta|\leq1}\cos(s\eta_n)\,d\eta. \end{gathered} \tag{B2} This is the exact flat Dirichlet density proved in Reflection and the Dirichlet boundary coefficient, Proposition 1.1. Radial integration, rather than differentiation of the rescaled profile, gives the useful uniform estimate Md′(k)=(2π)−nkn−1∫Sn−1[1−cos⁡(2dkθn)] dθ,0≤Md′(k)≤Cnkn−1,k>0.(B3) \begin{gathered} M_d'(k)\\ =(2\pi)^{-n}k^{n-1}\int_{S^{n-1}} [1-\cos(2dk\theta_n)]\,d\theta,\\ 0\leq M_d'(k)\leq C_n k^{n-1},\qquad k>0. \end{gathered} \tag{B3} The polar integration formula is proved in the coordinate and surface-measure reading. The integrand in (B3) lies between zero and two. Thus MdM_d is nondecreasing, is locally absolutely continuous across zero, and obeys 0≤Md(k)≤Cnkn0\leq M_d(k)\leq C_n k^n, uniformly for every d≥0d\geq0. The bounds involve no derivative in dd.

2. Fixed positive smoothing and a moderate weight

Fix any sufficiently small time T>0T>0. Choose an even nonnegative nonzero smooth function bb supported in (−T/2,T/2)(-T/2,T/2), and let vv be its inverse Fourier transform with convention f^(t)=∫e−itsf(s) ds\widehat f(t)=\int e^{-its}f(s)\,ds. Integration by parts shows that vv is Schwartz; it is real and even, and v(0)>0v(0)>0. Put ρ=v2/∫v2\rho=v^2/\int v^2. The Fourier product formula, proved by Fourier inversion and absolutely convergent integration for Schwartz functions in the Fourier reading, gives ρ≥0,ρ(−s)=ρ(s),∫ρ(s) ds=1,supp⁡ρ^⊂(−T,T),ca:=∫−aaρ(s) ds>0.(B4) \begin{gathered} \rho\geq0,\quad \rho(-s)=\rho(s),\\ \int\rho(s)\,ds=1,\quad \operatorname{supp}\widehat\rho\subset(-T,T),\\ c_a:=\int_{-a}^{a}\rho(s)\,ds>0. \end{gathered} \tag{B4} for some fixed a>0a>0. All constants may depend on this fixed kernel and on the operator and collar. They will not depend on x,d,kx,d,k.

Set Sx=ρ∗ExS_x=\rho*E_x and Sd0=ρ∗MdS_d^0=\rho*M_d. Their integrals converge by (B1)–(B3). For d>0d>0 define a weight on the whole real line by Bd(k)=(1+∣k∣)(1+∣k∣+d−1)n−2,(1+∣k∣)n−1≤Bd(k),Bd(k+s)≤Bd(k)(1+∣s∣)n−1.(B5) \begin{gathered} B_d(k)=(1+|k|)(1+|k|+d^{-1})^{n-2},\\ (1+|k|)^{n-1}\leq B_d(k),\\ B_d(k+s)\leq B_d(k)(1+|s|)^{n-1}. \end{gathered} \tag{B5} Indeed 1+∣k+s∣≤(1+∣k∣)(1+∣s∣)1+|k+s|\leq(1+|k|)(1+|s|) and 1+∣k+s∣+d−1≤(1+∣k∣+d−1)(1+∣s∣)1+|k+s|+d^{-1}\leq(1+|k|+d^{-1})(1+|s|). Multiplying proves the last line, with constant one. For k≥2k\geq2, Bd(k)B_d(k) is comparable to k(k+d−1)n−2k(k+d^{-1})^{n-2}, with constants depending only on nn.

The derivative estimate (B3), including the zero extension, implies ∣Md(k)−Md(k−s)∣≤C∣s∣(1+∣k∣+∣s∣)n−1,∣Sd0(k)−Md(k)∣≤C(1+∣k∣)n−1.(B6) \begin{gathered} |M_d(k)-M_d(k-s)|\\ \leq C|s|(1+|k|+|s|)^{n-1},\\ |S_d^0(k)-M_d(k)|\leq C(1+|k|)^{n-1}. \end{gathered} \tag{B6} For the first line integrate (B3) over the interval between the two arguments, intersected with the positive axis. For the second line integrate against ρ(s)\rho(s) and use its finite moments. These bounds are uniform even when dd tends to zero.

3. Removing smoothing without assuming a cluster bound

Theorem 3.1 (uniform cumulative Tauberian reduction). Suppose that for every point in the collar with d>0d>0, ∣Sx(k)−Sd0(k)∣≤CBd(k),k≥2,(B7) |S_x(k)-S_d^0(k)|\leq C B_d(k),\qquad k\geq2, \tag{B7} with one constant independent of the point. Then for either spectral endpoint convention, ∣Ex(k)−Md(k)∣≤C′Bd(k),k≥2,∣Ex(k)−Md(k)∣≤C′′kn,k≥2.(B8) \begin{gathered} |E_x(k)-M_d(k)|\leq C' B_d(k),\qquad k\geq2,\\ |E_x(k)-M_d(k)|\leq C'' k^n,\qquad k\geq2. \end{gathered} \tag{B8} At d=0d=0 both functions vanish. Conversely, the first estimate in (B8), uniformly for d>0d>0, implies (B7). Consequently the two-bound curved remainder is equivalent to (B7), given the already proved rough growth (B1).

Proof: low and negative frequencies. For any real k≤2k\leq2, (B1) bounds Sx(k)S_x(k) uniformly: the integrand is zero unless s≤ks\leq k, and then 1+k−s≤3+∣s∣1+k-s\leq3+|s|. Integrate Cρ(s)(3+∣s∣)nC\rho(s)(3+|s|)^n. The same argument applies to Sd0S_d^0. Since Bd≥1B_d\geq1, (B7) therefore holds on the whole real line after enlarging its constant. No uniform small-distance estimate is being assumed at low frequency.

A local mass estimate from cumulative differences. Put A=a+2A=a+2, where aa is from (B4). Positivity gives, for any real rr, caμx([r−1,r+1])≤Sx(r+A)−Sx(r−A)≤CBd(r).(B9) \begin{gathered} c_a\mu_x([r-1,r+1])\\ \leq S_x(r+A)-S_x(r-A)\\ \leq C B_d(r). \end{gathered} \tag{B9} For the first inequality, write the difference as the integral of Ex(r+A−s)−Ex(r−A−s)E_x(r+A-s)-E_x(r-A-s) against ρ(s)\rho(s). When ∣s∣≤a|s|\leq a, its lower endpoint is strictly below r−1r-1 and its upper endpoint strictly above r+1r+1. It therefore includes every atom in that closed interval for either convention. For other ss the difference is nonnegative. For the upper inequality replace both smoothed cumulative values by Sd0S_d^0, using (B7) and (B5). The model difference is bounded by C(1+∣r∣)n−1C(1+|r|)^{n-1}: integrate (B3) over an interval of length 2A2A, then against ρ\rho. This is bounded by CBd(r)C B_d(r) by (B5). Thus (B9) is derived, not an extra spectral-cluster hypothesis.

Cover the interval between kk and k−sk-s by at most C(1+∣s∣)C(1+|s|) closed intervals of radius one, whose centers lie within ∣s∣+1|s|+1 of kk. The variation of either cumulative convention between the two endpoints is bounded by the measure of that closed interval. Equations (B9) and (B5) give ∣Ex(k)−Ex(k−s)∣≤CBd(k)(1+∣s∣)n,∣Ex(k)−Sx(k)∣≤CBd(k).(B10) \begin{gathered} |E_x(k)-E_x(k-s)| \leq C B_d(k)(1+|s|)^n,\\ |E_x(k)-S_x(k)|\leq C B_d(k). \end{gathered} \tag{B10} The second line follows by integration against the positive Schwartz kernel. It also controls an atom exactly at kk, so no continuity of the spectral staircase was assumed. Combining (B10), (B7) and (B6) proves the first part of (B8). The second part follows directly from (B1) and (B3), since k≥2k\geq2. Every Dirichlet eigenfunction is smooth and zero at the wall, so Ex=0E_x=0 there; (B2) gives M0=0M_0=0.

For the converse, extend the assumed bound for Ex−MdE_x-M_d to all real arguments: both vanish at negative arguments, and their difference is uniformly bounded on [0,2][0,2] by (B1) and (B3). Convolve this bound and use (B5) and the finite (n−1)(n-1)-st moment of ρ\rho. This proves (B7). □\square

4. The exact short-time quantity to estimate

The uniform growth permits us to define the diagonal cosine distribution directly by Cx(t)=∫0∞cos⁡(tκ) dμx(κ),Cd0(t)=∫0∞cos⁡(tκ) dMd(κ).(B11) \begin{gathered} C_x(t)=\int_0^\infty\cos(t\kappa)\,d\mu_x(\kappa),\\ C_d^0(t)=\int_0^\infty\cos(t\kappa)\,dM_d(\kappa). \end{gathered} \tag{B11} These are distributional integrals. Pairing with a Schwartz test function gives rapidly decreasing Fourier transforms in κ\kappa. Splitting the positive axis into unit intervals and using (B1) or (B3) proves absolute convergence, bounded by finitely many Schwartz seminorms uniformly in x,dx,d. Thus (B11) defines tempered distributions without requiring an unproved pullback of a singular kernel to the diagonal. It is the time-tested spectral definition of the diagonal of cos⁡(tP)\cos(t\sqrt P). The pairing below is linear, without complex conjugation on the test function.

Let F(z)=∫−∞zρ(s) dsF(z)=\int_{-\infty}^z\rho(s)\,ds. Positivity and interchange of the two integrals give Sx(k)=∫0∞F(k−κ) dμx(κ).(B12) S_x(k)=\int_0^\infty F(k-\kappa)\,d\mu_x(\kappa). \tag{B12} The strict and closed conventions have the same convolution: for each fixed atom the excluded endpoint is a single integration value, of Lebesgue measure zero. The same formula holds for Sd0S_d^0, with dMddM_d.

Theorem 4.1 (cosine formula and uniform tail). For k≥2k\geq2, Sx(k)=1π⟨Cx(t),ρ^(t)sin⁡(kt)t⟩+Tx(k),Tx(k)=∫0∞[1−F(k+κ)] dμx(κ),0≤Tx(k)≤CNk−Nfor every N.(B13) \begin{gathered} S_x(k)=\frac1\pi \left\langle C_x(t),\widehat\rho(t)\frac{\sin(kt)}t\right\rangle +T_x(k),\\ T_x(k)=\int_0^\infty[1-F(k+\kappa)]\,d\mu_x(\kappa),\\ 0\leq T_x(k)\leq C_N k^{-N}\quad\text{for every }N. \end{gathered} \tag{B13} The constants are uniform up to the boundary. There is an identical formula and estimate for Sd0,Cd0,Td0S_d^0,C_d^0,T_d^0, uniform in d≥0d\geq0.

Proof. Fourier inversion and evenness of ρ\rho give, for one frequency κ≥0\kappa\geq0, 1π∫cos⁡(tκ)ρ^(t)sin⁡(kt)t dt=∫0k[ρ(s−κ)+ρ(s+κ)] ds=F(k−κ)+F(k+κ)−1.(B14) \begin{gathered} \frac1\pi\int\cos(t\kappa)\widehat\rho(t) \frac{\sin(kt)}t\,dt\\ =\int_0^k[\rho(s-\kappa)+\rho(s+\kappa)]\,ds\\ =F(k-\kappa)+F(k+\kappa)-1. \end{gathered} \tag{B14} Here sin⁡(kt)/t=∫0kcos⁡(st) ds\sin(kt)/t=\int_0^k\cos(st)\,ds, with value kk at zero. The factor 1/π1/\pi follows from the inverse Fourier factor 1/(2π)1/(2\pi) and the sum of the two even frequencies. The identity F(−κ)+F(κ)=1F(-\kappa)+F(\kappa)=1 gives the final constant.

The test function ρ^(t)sin⁡(kt)/t\widehat\rho(t)\sin(kt)/t is smooth and supported in (−T,T)(-T,T). For fixed kk, its cosine transform decays faster than any inverse power of κ\kappa; hence (B11) allows its termwise pairing. Alternatively both expressions on the last line of (B14), after writing it as F(k−κ)−[1−F(k+κ)]F(k-\kappa)-[1-F(k+\kappa)], are absolutely integrable against the polynomially growing positive measure. Integration of (B14) therefore proves (B13).

For the tail, 1−F(z)≤CL(1+z)−L1-F(z)\leq C_L(1+z)^{-L} for z≥0z\geq0. The mass of [m,m+1][m,m+1] is at most C(m+2)nC(m+2)^n, uniformly in the point, by (B1). Counting shared endpoints twice only enlarges the positive bound. Consequently Tx(k)≤CL∑m=0∞(m+2)n(k+m)−L≤CL′kn+1−L,L>n+1.(B15) \begin{gathered} T_x(k)\leq C_L\sum_{m=0}^\infty (m+2)^n(k+m)^{-L}\\ \leq C_L' k^{n+1-L},\qquad L>n+1. \end{gathered} \tag{B15} For the last inequality split at m≤km\leq k; the first sum has at most k+1k+1 terms bounded by Ckn−LC k^{n-L}, and the remaining power sum is bounded by its convergent integral. Choose L≥N+n+1L\geq N+n+1, increasing it strictly above n+1n+1 if needed. Equation (B3) gives the same interval-mass bound for the model. □\square

Combining the two theorems yields an exact reduction of the required curved estimate. It suffices, and is necessary up to a change of constant, to prove ∣1π⟨Cx−Cd0,ρ^(t)sin⁡(kt)t⟩∣≤CBd(k),k≥2, d>0.(B16) \begin{gathered} \left|\frac1\pi\left\langle C_x-C_d^0, \widehat\rho(t)\frac{\sin(kt)}t\right\rangle\right|\\ \leq C B_d(k),\qquad k\geq2,\ d>0. \end{gathered} \tag{B16} The rapid tails in (B13) are absorbed because Bd≥1B_d\geq1. With h=k−1h=k^{-1}, the size required on the right is comparable to h1−n(1+h/d)n−2.(B17) h^{1-n}(1+h/d)^{n-2}. \tag{B17} This reduction retains the metric-volume normalization and the full operator scope. Knowledge of the wavefront relation alone does not estimate (B16).

5. A quantitative reflected-phase freezing lemma

Here the distance dd is a smooth parameter; this section is an oscillatory-integral lemma, with no assumed representation of the actual kernel. Fix 0<E0<10<E_0<1. Let yy range over a compact parameter set, let 0≤d≤d00\leq d\leq d_0, and let ζ∈Rn−1\zeta\in\mathbb R^{n-1}. Suppose the real phase ϕ(d,y,ζ,E)\phi(d,y,\zeta,E) and amplitude A(d,y,ζ,E)A(d,y,\zeta,E) are smooth for E∈[E0,1]E\in[E_0,1]. The amplitude has uniformly compact ζ\zeta-support and vanishes in a fixed neighborhood of E0E_0. On a fixed neighborhood of its support suppose there is a smooth single critical branch ζc(d,y,E)\zeta_c(d,y,E), with uniformly invertible ζ\zeta-Hessian. Away from a fixed neighborhood of this branch, assume ∣∂ζϕ∣|\partial_\zeta\phi| has a positive uniform lower bound on the support. Assume, crucially, ϕ(d,y,ζc(d,y,E),E)=Φ(y,E),∣∂EΦ(y,E)∣≥c>0.(B18) \begin{gathered} \phi(d,y,\zeta_c(d,y,E),E)=\Phi(y,E),\\ |\partial_E\Phi(y,E)|\geq c>0. \end{gathered} \tag{B18} Thus the critical action is independent of dd. All necessary finite derivatives and inverse-Hessian bounds are uniform on the compact parameter set. Finitely many branches can be treated by a fixed partition and addition. Uniform extra parameters in the amplitudes are allowed with the same bounds.

Define, for r>0r>0, J(d,y,r)=∫E01I(d,y,E,r) dE,I(d,y,E,r)=∫Rn−1eirϕ(d,y,ζ,E)A(d,y,ζ,E) dζ.(B19) \begin{gathered} J(d,y,r)=\int_{E_0}^1 I(d,y,E,r)\,dE,\\ I(d,y,E,r)\\ =\int_{\mathbb R^{n-1}}e^{ir\phi(d,y,\zeta,E)} A(d,y,\zeta,E)\,d\zeta. \end{gathered} \tag{B19}

Lemma 5.1 (fixed-action freezing). Under these hypotheses, ∣J(d,y,r)−J(0,y,r)∣≤Cdmin⁡{1,r−(n+1)/2}.(B20) \begin{gathered} |J(d,y,r)-J(0,y,r)|\\ \leq C d\min\{1,r^{-(n+1)/2}\}. \end{gathered} \tag{B20} In particular, for 0<h≤10<h\leq1, uniformly in 0<d≤d00<d\leq d_0, h−n∣J(d,y,d/h)−J(0,y,d/h)∣≤Ch1−n.(B21) h^{-n}|J(d,y,d/h)-J(0,y,d/h)|\leq C h^{1-n}. \tag{B21}

Proof. For 0<r≤10<r\leq1, differentiate the integrand in dd. The derivative is eirϕ(∂dA+irA∂dϕ)e^{ir\phi}(\partial_d A+irA\partial_d\phi), whose integral is uniformly bounded because the integration region is fixed and compact. The fundamental theorem of calculus on [0,d][0,d] proves (B20) in this range.

For r≥1r\geq1, apply the parameter Morse and stationary-phase proof cited above, in m=n−1m=n-1 variables, with parameters (d,y,E)(d,y,E). After removing the critical exponential it gives an exact representation I(d,y,E,r)=eirΦ(y,E)b(d,y,E,r),∣∂da∂Ejb(d,y,E,r)∣≤Ca,jr−(n−1)/2,a,j∈{0,1}.(B22) \begin{gathered} I(d,y,E,r)=e^{ir\Phi(y,E)}b(d,y,E,r),\\ |\partial_d^a\partial_E^j b(d,y,E,r)| \leq C_{a,j}r^{-(n-1)/2},\\ a,j\in\{0,1\}. \end{gathered} \tag{B22} These bounds include the mixed derivative. To see explicitly why the remainder has this property, use the smooth Morse coordinates of (P1) to replace the phase near the branch by its critical value plus a fixed nondegenerate quadratic form. The Jacobian and transformed amplitude have uniform parameter derivatives. Equations (P4)–(P8) give the asserted bounds for this quadratic integral. On the complement, repeated integration by parts using (P10) gives arbitrary decay even after differentiating in d,Ed,E and removing eirΦe^{ir\Phi}; any finitely many extra powers of rr are absorbed by additional integrations. A finite parameter cover gives the uniform constants. This also shows that bb vanishes near E0E_0. No derivative of a moving critical exponential is hidden in (B22).

Put D(E)=b(d,y,E,r)−b(0,y,E,r)D(E)=b(d,y,E,r)-b(0,y,E,r). Integration of the dd-derivative in (B22) gives ∣D∣+∣∂ED∣≤Cdr−(n−1)/2|D|+|\partial_E D|\leq C d r^{-(n-1)/2}. Because the same Φ\Phi occurs at both distances, integration by parts in energy gives J(d,y,r)−J(0,y,r)=[eirΦDir∂EΦ]E01−1ir∫E01eirΦ∂E ⁣(D∂EΦ)dE.(B23) \begin{gathered} J(d,y,r)-J(0,y,r)\\ =\left[\frac{e^{ir\Phi}D}{ir\partial_E\Phi}\right]_{E_0}^1\\ -\frac1{ir}\int_{E_0}^1 e^{ir\Phi} \partial_E\!\left(\frac D{\partial_E\Phi}\right)dE. \end{gathered} \tag{B23} The lower endpoint is zero; the upper endpoint is retained. The lower bound in (B18) and bounded second energy derivative of Φ\Phi prove the remaining part of (B20).

For (B21), if d≤hd\leq h, use h−nd≤h1−nh^{-n}d\leq h^{1-n}. If d≥hd\geq h, the other part of (B20) gives h−nd(h/d)(n+1)/2=h1−n(h/d)(n−1)/2≤h1−n.(B24) \begin{gathered} h^{-n}d(h/d)^{(n+1)/2}\\ =h^{1-n}(h/d)^{(n-1)/2}\leq h^{1-n}. \end{gathered} \tag{B24} The comparison is zero at d=0d=0 by its definition before substitution. This completes the proof. □\square

The fixed-action assumption is substantial. Even a difference of order dd between critical values can produce an additional factor rdrd when exponentials are subtracted. Smooth coefficients alone therefore do not justify (B20). For the actual boundary kernel one must construct the relevant phase patches, identify the common critical action, verify the parameter bounds, handle all other patches, and control the exact operator remainder in (B16). A formal frozen amplitude is not that construction.

6. Constructing the two phases from the metric

Write a boundary normal chart as (a,z)(a,z), where a≥0a\geq0 is distance and z∈Rn−1z\in\mathbb R^{n-1}. Reserve (d,y)(d,y) for the source point. On a compact chart inside a larger one the actual principal symbol is p(a,z,s,ζ)=s2+r(a,z,ζ),r(a,z,ζ)=ζTG(a,z)ζ,λσ(a,z,ζ,E)=σE−r(a,z,ζ),σ=±1.(B25) \begin{gathered} p(a,z,s,\zeta)=s^2+r(a,z,\zeta),\\ r(a,z,\zeta)=\zeta^{\mathsf T}G(a,z)\zeta,\\ \lambda_\sigma(a,z,\zeta,E)\\ =\sigma\sqrt{E-r(a,z,\zeta)},\qquad\sigma=\pm1. \end{gathered} \tag{B25} Here GG is real symmetric and uniformly positive. Fix 0<E0<10<E_0<1. For E∈[E0,1]E\in[E_0,1], choose a small tangential frequency ball and a short fixed collar so that E−r≥E0/2E-r\geq E_0/2 on a slightly larger region. Every derivative of both roots is bounded there, uniformly in all parameters. Smoothness up to the wall permits an auxiliary smooth extension for local inverse arguments at zero; none of the asserted equations uses a physical point outside the collar.

We construct an incident phase SσiS^i_\sigma from the source normal slice, and a reflected phase SσrS^r_\sigma from the wall: ∂aSσi=λσ(a,z,∂zSσi,E),Sσi(d,z;d,y,η,E)=(z−y)⋅η,∂aSσr=λσ(a,z,∂zSσr,E),Sσr(0,z;d,y,η,E)=S−σi(0,z;d,y,η,E).(B26) \begin{gathered} \partial_a S^i_\sigma =\lambda_\sigma(a,z,\partial_z S^i_\sigma,E),\\ S^i_\sigma(d,z;d,y,\eta,E)=(z-y)\cdot\eta,\\ \partial_a S^r_\sigma =\lambda_\sigma(a,z,\partial_z S^r_\sigma,E),\\ S^r_\sigma(0,z;d,y,\eta,E) =S^i_{-\sigma}(0,z;d,y,\eta,E). \end{gathered} \tag{B26} Both phases are real and smooth jointly in all variables for 0≤a,d≤d00\leq a,d\leq d_0, y,zy,z in retained chart neighborhoods, small η\eta, and E∈[E0,1]E\in[E_0,1]. The same neighborhood works at d=0d=0. The matching phases at the wall are equal; Dirichlet cancellation will put a minus sign in the amplitudes.

Here is the construction and its uniformity. For any smooth initial function f(w)f(w) on the slice a=a0a=a_0, solve Z′=−∂ζλσ(a,Z,Ξ,E),Ξ′=∂zλσ(a,Z,Ξ,E),Z(a0)=w,Ξ(a0)=df(w),s(a)=f(w)+∫a0aΞ(v)⋅Z′(v) dv+∫a0aλσ(v,Z(v),Ξ(v),E) dv.(B27) \begin{gathered} Z'=-\partial_\zeta\lambda_\sigma(a,Z,\Xi,E),\\ \Xi'=\partial_z\lambda_\sigma(a,Z,\Xi,E),\\ Z(a_0)=w,\qquad \Xi(a_0)=df(w),\\ s(a)=f(w)+\int_{a_0}^{a}\Xi(v)\cdot Z'(v)\,dv\\ +\int_{a_0}^{a}\lambda_\sigma(v,Z(v),\Xi(v),E)\,dv. \end{gathered} \tag{B27} The contraction and differentiated integral-equation proof in Existence and compactness of generalized reflected curves, equation (G13), supplies this smooth flow with smooth dependence on the initial slice and every displayed parameter. Its constants are uniform on the larger compact region. At a=a0a=a_0, the derivative ZwZ_w is the identity. Bounded differentiated flow equations therefore give Zw=I+O(∣a−a0∣)Z_w=I+O(|a-a_0|) for the bounded initial families used here. Choose the collar once so that this matrix stays invertible. The parameter inverse proof then solves Z(a,w)=zZ(a,w)=z smoothly for ww.

Define S(a,z)=s(a,w(a,z))S(a,z)=s(a,w(a,z)). Varying ww under the action integral shows dws(a)=Ξ(a)dwZ(a)d_ws(a)=\Xi(a)d_wZ(a): the variation of its integrand is the derivative of Ξ⋅δZ\Xi\cdot\delta Z, because Z′=−λζZ'=-\lambda_\zeta and Ξ′=λz\Xi'=\lambda_z; its initial endpoint cancels df=Ξ(a0)dwdf=\Xi(a_0)dw. It follows that ∂zS=Ξ(a,w(a,z)),∂aS=λσ(a,z,∂zS,E).(B28) \begin{gathered} \partial_zS=\Xi(a,w(a,z)),\\ \partial_aS=\lambda_\sigma(a,z,\partial_zS,E). \end{gathered} \tag{B28} The second identity follows by differentiating Z(a,w(a,z))=zZ(a,w(a,z))=z at fixed zz, so the action's Ξ⋅Z′\Xi\cdot Z' term cancels. Conversely, the gradient of any solution of this initial problem follows (B27), by differentiating its equation. Flow uniqueness and the initial value give uniqueness of SS.

First apply this construction to f(w)=(w−y)⋅ηf(w)=(w-y)\cdot\eta and a0=da_0=d. Its parameter derivatives are bounded. Then take the resulting smooth boundary value f(w)=S−σi(0,w;d,y,η,E)f(w)=S^i_{-\sigma}(0,w;d,y,\eta,E) and a0=0a_0=0. Its first two spatial derivatives are uniformly bounded and its gradient stays in the larger root region after reducing the collar. The construction applies again. Finite covers of a compact boundary chart give one common collar and frequency radius. This proves (B26), including all parameter derivatives and the normal-root gap; no formal eikonal solution is being assumed.

7. The exact critical action and Hessian on the diagonal

Put Θσ(d,y,η,E)=Sσr(d,y;d,y,η,E)\Theta_\sigma(d,y,\eta,E)=S^r_\sigma(d,y;d,y,\eta,E). Since Θσ(0,y,η,E)=0\Theta_\sigma(0,y,\eta,E)=0, its normalized phase extends smoothly through zero: ψσ(d,y,η,E)=∫01∂dΘσ(vd,y,η,E) dv,Θσ=dψσ,ψσ(0,y,η,E)=2σE−ηTG(0,y)η.(B29) \begin{gathered} \psi_\sigma(d,y,\eta,E) =\int_0^1\partial_d\Theta_\sigma(vd,y,\eta,E)\,dv,\\ \Theta_\sigma=d\psi_\sigma,\\ \psi_\sigma(0,y,\eta,E) =2\sigma\sqrt{E-\eta^{\mathsf T}G(0,y)\eta}. \end{gathered} \tag{B29} The last equality follows by differentiating (B26) when both normal slices are zero. The target-slice derivative contributes λσ\lambda_\sigma. The derivative of the incident initial slice contributes −λ−σ-\lambda_{-\sigma}, because differentiation of S−σi(d,z;d,y,η,E)=(z−y)⋅ηS^i_{-\sigma}(d,z;d,y,\eta,E)=(z-y)\cdot\eta gives ∂dS−σi=−∂aS−σi\partial_d S^i_{-\sigma}=-\partial_a S^i_{-\sigma} there. Their sum is 2λσ2\lambda_\sigma. The first formula in (B29), which is Taylor's integral identity in the single distance variable, also proves every uniform derivative bound after division by dd.

At η=0\eta=0, the incident and reflected solutions and their first frequency derivatives are particularly simple: Sσi(a,z;d,y,0,E)=σ(a−d)E,Sσr(a,z;d,y,0,E)=σ(a+d)E,∂ηSσi∣η=0=z−y,∂ηSσr∣η=0=z−y.(B30) \begin{gathered} S^i_\sigma(a,z;d,y,0,E)=\sigma(a-d)\sqrt E,\\ S^r_\sigma(a,z;d,y,0,E)=\sigma(a+d)\sqrt E,\\ \left.\partial_\eta S^i_\sigma\right|_{\eta=0}=z-y, \qquad \left.\partial_\eta S^r_\sigma\right|_{\eta=0}=z-y. \end{gathered} \tag{B30} Indeed the first two expressions solve (B26), since the root at zero tangential momentum is σE\sigma\sqrt E, independent of a,za,z. Uniqueness proves them. Differentiating the eikonal equation once in η\eta gives ∂aSη=λζSzη\partial_a S_\eta=\lambda_\zeta S_{z\eta}. At η=0\eta=0 its right side vanishes, so its prescribed initial value z−yz-y remains unchanged on each leg. Thus ψσ(d,y,0,E)=2σE,∂ηψσ(d,y,0,E)=0,∂Eψσ(d,y,0,E)=σ/E.(B31) \begin{gathered} \psi_\sigma(d,y,0,E)=2\sigma\sqrt E,\\ \partial_\eta\psi_\sigma(d,y,0,E)=0,\\ \partial_E\psi_\sigma(d,y,0,E)=\sigma/\sqrt E. \end{gathered} \tag{B31} These identities include d=0d=0 by (B29). In particular the critical action is exactly independent of distance, rather than just constant to first order.

The Hessian is also explicit. Define the positive matrix G‾(d,y)=∫01G(vd,y) dv\overline G(d,y)=\int_0^1G(vd,y)\,dv. Differentiating the eikonal equation twice and using Szη=IS_{z\eta}=I from (B30) gives ∂aSηη=λζζ(a,z,0,E)=−σG(a,z)/E\partial_a S_{\eta\eta}=\lambda_{\zeta\zeta}(a,z,0,E)=-\sigma G(a,z)/\sqrt E on the σ\sigma leg. The incident −σ-\sigma leg starts with zero Hessian on a=da=d; its backward integral from dd to zero is −σE−1/2∫0dG(v,z) dv-\sigma E^{-1/2}\int_0^dG(v,z)\,dv. The reflected σ\sigma leg adds the same integral on its forward journey to a=da=d. Consequently ∂η2ψσ(d,y,0,E)=−2σE G‾(d,y),G‾(0,y)=G(0,y),G‾(d,y)≥cGI.(B32) \begin{gathered} \partial_\eta^2\psi_\sigma(d,y,0,E) =-\frac{2\sigma}{\sqrt E}\,\overline G(d,y),\\ \overline G(0,y)=G(0,y),\qquad \overline G(d,y)\geq c_G I. \end{gathered} \tag{B32} This calculation differentiates at fixed target coordinate zz before setting z=yz=y; it does not identify a moving coordinate with that fixed derivative.

Smoothness of ψσ\psi_\sigma, compactness of the parameter range and (B32) give, on one sufficiently small frequency ball, −σ∂η2ψσ≥cI,∣∂ηψσ(d,y,η,E)∣≥c∣η∣.(B33) \begin{gathered} -\sigma\partial_\eta^2\psi_\sigma\geq cI,\\ |\partial_\eta\psi_\sigma(d,y,\eta,E)|\geq c|\eta|. \end{gathered} \tag{B33} For the second inequality, integrate the Hessian on the segment from zero to η\eta, pair with −ση-\sigma\eta, and use (B31) and Cauchy–Schwarz. Hence zero is the unique critical point in that ball, the Hessian has signature −σ(n−1)-\sigma(n-1), and the phase is uniformly nonstationary outside any smaller ball. Since ∣σ/E∣≥1|\sigma/\sqrt E|\geq1 on the chosen energy interval, all hypotheses (B18) of the fixed-action freezing lemma are now verified for these actual metric phases. This assertion concerns these near-normal phases, not a representation of every part of the spectral kernel.

8. Transport with the actual lower-order terms

Represent a half density by its scalar coefficient relative to ∣da dz∣1/2|da\,dz|^{1/2}. In this representation the actual differential expression has the form P=∑j,k=1ngjk(a,z)DjDk+∑j=1nbj(a,z)Dj+c(a,z),Dj=−i∂j,(gjk)=(100G).(B34) \begin{gathered} P=\sum_{j,k=1}^n g^{jk}(a,z)D_jD_k\\ +\sum_{j=1}^n b_j(a,z)D_j+c(a,z),\\ D_j=-i\partial_j,\qquad (g^{jk})=\begin{pmatrix}1&0\\0&G\end{pmatrix}. \end{gathered} \tag{B34} The smooth coefficients bj,cb_j,c include all ordering and lower-order terms; they need not be real in left quantization. Nothing in the following construction discards them or assumes a Laplace operator.

For any one of the phases in (B26), direct differentiation of the degree-two differential expression gives the exact identity e−iS/h(h2P−E)(eiS/hA)=hTSA+h2PA.(B35) \begin{gathered} e^{-iS/h}(h^2P-E)(e^{iS/h}A)\\ =h\mathcal T_S A+h^2PA. \end{gathered} \tag{B35} where TSA=2i∑j,kgjkSj∂kA+1i∑j,kgjkSjkA+(∑jbjSj)A.(B36) \begin{aligned} \mathcal T_S A={}&\frac2i\sum_{j,k}g^{jk}S_j\partial_kA\\ &+\frac1i\sum_{j,k}g^{jk}S_{jk}A\\ &+\left(\sum_j b_jS_j\right)A. \end{aligned} \tag{B36} The eikonal equation cancels (p(dS)−E)A(p(dS)-E)A. The coefficient of ∂aA\partial_a A in TS\mathcal T_S is 2Sa/i2S_a/i, uniformly separated from zero. After division by that coefficient, the transport equation is an ordinary scalar equation along the base characteristics with velocity GSz/Sa=−∂ζλσ(a,z,Sz,E)G S_z/S_a=-\partial_\zeta\lambda_\sigma(a,z,S_z,E). These are precisely the projected characteristics used above.

For every integer L≥0L\geq0, choose smooth bounded initial coefficient functions gσ,j(z;d,y,η,E)g_{\sigma,j}(z;d,y,\eta,E), 0≤j≤L0\leq j\leq L, supported in the retained frequency and energy region. Prescribe incident coefficients on a=da=d, and reflected coefficients on a=0a=0, by TSa0=0,TSaj=−Paj−1(1≤j≤L),aσ,ji(d,z;d,y,η,E)=gσ,j(z;d,y,η,E),aσ,jr(0,z;d,y,η,E)=−a−σ,ji(0,z;d,y,η,E).(B37) \begin{gathered} \mathcal T_S a_0=0,\\ \mathcal T_S a_j=-P a_{j-1}\quad(1\leq j\leq L),\\ a^i_{\sigma,j}(d,z;d,y,\eta,E)\\ =g_{\sigma,j}(z;d,y,\eta,E),\\ a^r_{\sigma,j}(0,z;d,y,\eta,E)\\ =-a^i_{-\sigma,j}(0,z;d,y,\eta,E). \end{gathered} \tag{B37} Solve the incident recursion first and then the reflected one. To justify every step, write its divided equation along a characteristic as u′+qu=fu'+q u=f. Multiplication by e∫qe^{\int q} gives u(a)=e−∫a0aq[u(a0)+∫a0ae∫a0vqf(v) dv]u(a)=e^{-\int_{a_0}^a q}[u(a_0)+\int_{a_0}^a e^{\int_{a_0}^v q}f(v)\,dv]. Differentiation verifies the equation and initial value, with oriented integrals for a backward incident leg. The intervals are uniformly bounded, their coefficients and all parameter derivatives are bounded, and the flow inverse is uniformly smooth. Differentiating this formula proves all parameter bounds. At each recursion step Paj−1P a_{j-1} uses only the already obtained smooth derivatives. This proves existence, uniqueness and uniform bounds for all finite coefficient families, including mixed derivatives in the source distance dd through zero. No expansion or division in that distance is used in the transport equations.

Set Aσ,Li=∑j=0Lhjaσ,jiA^i_{\sigma,L}=\sum_{j=0}^Lh^j a^i_{\sigma,j}, and define Aσ,LrA^r_{\sigma,L} in the same way. Equations (B35)–(B37) telescope to (h2P−E)(eiS/hAL)=hL+2eiS/hPaL,eiS−σi/hA−σ,Li+eiSσr/hAσ,Lr∣a=0=0.(B38) \begin{gathered} (h^2P-E)(e^{iS/h}A_L) =h^{L+2}e^{iS/h}P a_L,\\ \left.e^{iS^i_{-\sigma}/h}A^i_{-\sigma,L} +e^{iS^r_\sigma/h}A^r_{\sigma,L}\right|_{a=0}=0. \end{gathered} \tag{B38} The boundary cancellation is exact for every h>0h>0. In the frozen flat case the phases are (z−y)η−σ(a−d)E−r0(η)(z-y)\eta-\sigma(a-d)\sqrt{E-r_0(\eta)} and (z−y)η+σ(a+d)E−r0(η)(z-y)\eta+\sigma(a+d)\sqrt{E-r_0(\eta)}; they agree at a=0a=0. This also checks the reflection sign directly.

Frequency and energy supports of the coefficients are retained by the recursion: its differentiations are in (a,z)(a,z), and the characteristic parameter (η,E)(\eta,E) is fixed. A fixed energy cutoff vanishing near E0E_0 can therefore be built into the initial coefficients. Initial base supports can be chosen strictly inside the chart so that their two transported supports stay inside the larger chart. Alternatively every estimate can be restricted to a compact subchart where an auxiliary base cutoff is one. Derivatives of a subsequently imposed base cutoff are separate commutator errors on its transition region; (B38) does not call those errors small.

9. Quantitative residuals and the frozen diagonal family

For a fixed choice ε=±1\varepsilon=\pm1, form the finite wave-phase integral Vσ,L=eiS−σi/hA−σ,Li+eiSσr/hAσ,Lr,Kh,L(t,a,z;d,y)=(2πh)−n∑σ=±1∫E01∫eitεE/hVσ,L dη dE.(B39) \begin{gathered} \mathcal V_{\sigma,L}=e^{iS^i_{-\sigma}/h}A^i_{-\sigma,L} +e^{iS^r_\sigma/h}A^r_{\sigma,L},\\ K_{h,L}(t,a,z;d,y)\\ =(2\pi h)^{-n}\sum_{\sigma=\pm1}\int_{E_0}^1\int e^{it\varepsilon\sqrt E/h}\mathcal V_{\sigma,L}\,d\eta\,dE. \end{gathered} \tag{B39} The amplitudes have uniformly compact η\eta-support. They may be nonzero at the upper energy endpoint. This causes no problem when applying a differential operator or taking a fixed ordinary parameter derivative under the finite integral. With Qh=(hDt)2−h2PQ_h=(hD_t)^2-h^2P, (B38) gives, on the retained compact charts and any fixed bounded time interval, Kh,L∣a=0=0,∣∂αQhKh,L∣≤CL,αhL+2−n−∣α∣.(B40) \begin{gathered} K_{h,L}|_{a=0}=0,\\ |\partial^\alpha Q_h K_{h,L}| \leq C_{L,\alpha}h^{L+2-n-|\alpha|}. \end{gathered} \tag{B40} Here ∂α\partial^\alpha may differentiate time, target coordinates or source coordinates. Each derivative of an exponential costs at most one power of h−1h^{-1}; all phase derivatives and amplitude derivatives are uniformly bounded. The un-differentiated residual is exactly the integral of −hL+2ei(tεE+S)/hPaL-h^{L+2}e^{i(t\varepsilon\sqrt E+S)/h}Pa_L. Its absolute integral, and the same calculation after differentiating, prove (B40). Thus any prescribed finite number of derivatives and any prescribed residual power can be attained by increasing LL. The construction has not yet imposed the physical Cauchy data that identify this family with the actual cosine kernel.

For density normalization write dVg=γ(a,z) da dz,γ(a,z)=(det⁡G(a,z))−1/2.(B41) \begin{gathered} dV_g=\gamma(a,z)\,da\,dz,\\ \gamma(a,z)=(\det G(a,z))^{-1/2}. \end{gathered} \tag{B41} A coordinate half-density kernel has scalar diagonal relative to dVgdV_g equal to its coordinate diagonal divided by γ\gamma. Indeed v∣da dz∣1/2=u(dVg)1/2v|da\,dz|^{1/2}=u(dV_g)^{1/2} means u=γ−1/2vu=\gamma^{-1/2}v; apply this to both kernel factors. The smooth positive factors γ±1\gamma^{\pm1} and all their derivatives are bounded on the retained collar.

Consider the reflected diagonal family aσ,Ldiag(d,y,η,E)=γ(d,y)−1Aσ,Lr(d,y;d,y,η,E),Fh,L(d,y)=(2πh)−n∑σ∫E01∫eidψσ/haσ,Ldiag dη dE.(B42) \begin{gathered} a^{\rm diag}_{\sigma,L}(d,y,\eta,E)\\ =\gamma(d,y)^{-1}A^r_{\sigma,L}(d,y;d,y,\eta,E),\\ F_{h,L}(d,y)\\ =(2\pi h)^{-n}\sum_\sigma\int_{E_0}^1\int e^{id\psi_\sigma/h}a^{\rm diag}_{\sigma,L}\,d\eta\,dE. \end{gathered} \tag{B42} Let Fh0(d,y)F_h^0(d,y) be the same expression keeping only j=0j=0, and replacing the smooth distance parameters in ψ,γ,a0r\psi,\gamma,a^r_0 by zero, while retaining d/hd/h in the exponential. Then ∣Fh,L(d,y)−Fh0(d,y)∣≤CLh1−n,0≤d≤d0.(B43) \begin{gathered} |F_{h,L}(d,y)-F_h^0(d,y)|\\ \leq C_Lh^{1-n},\qquad 0\leq d\leq d_0. \end{gathered} \tag{B43} To prove this, apply Lemma 5.1 to each actual metric phase ψσ\psi_\sigma. Its hypotheses were verified in (B29)–(B33), and (B37) supplies all required distance and energy derivatives of the amplitude, including the factor γ−1\gamma^{-1}. The lower energy cutoff makes that amplitude vanish near E0E_0. This gives the claimed bound for the leading term. Every higher term is bounded directly by Cjhj−nC_jh^{j-n}, using its compact integration region, so their finite sum is O(h1−n)O(h^{1-n}). At d=0d=0 the leading difference vanishes and the same estimate for the higher terms applies. This proves a uniform coefficient-freezing bound for the constructed family, including arbitrary smooth lower-order coefficients.

Its frozen normalization can be fixed explicitly. Suppose the leading incident seeds on the zero source slice satisfy, at z=yz=y, gσ,0(y;0,y,η,E)=χ(E)β(y,η,E)2E−r(0,y,η).(B44) g_{\sigma,0}(y;0,y,\eta,E) =\frac{\chi(E)\beta(y,\eta,E)} {2\sqrt{E-r(0,y,\eta)}}. \tag{B44} Here χ\chi vanishes near E0E_0, and β\beta is supported in the small near-normal frequency ball. Smooth such seed families exist because the denominator is separated from zero; multiply by an initial base cutoff equal to one near z=yz=y and extend in dd using the same positive root. By (B37), the reflected leading coefficient at zero is the negative of (B44). Thus λ0(y,η,E)=E−r(0,y,η),Fh0(d,y)=−(2πh)−nγ(0,y)∑σ=±1∫E01∫e2iσdλ0/hχ(E)β(y,η,E)2λ0 dη dE.(B45) \begin{gathered} \lambda_0(y,\eta,E)=\sqrt{E-r(0,y,\eta)},\\ F_h^0(d,y)=-\frac{(2\pi h)^{-n}}{\gamma(0,y)} \sum_{\sigma=\pm1}\int_{E_0}^1\int\\ \quad e^{2i\sigma d\lambda_0/h} \frac{\chi(E)\beta(y,\eta,E)}{2\lambda_0}\,d\eta\,dE. \end{gathered} \tag{B45} This is precisely the corresponding part of the frozen reflected phase-volume integral. For each fixed η\eta, use the two branches s=σE−r(0,y,η)s=\sigma\sqrt{E-r(0,y,\eta)}; the positive Jacobian is ∣ds/dE∣=1/(2E−r)|ds/dE|=1/(2\sqrt{E-r}). This proves (B45)'s normalization and its negative Dirichlet sign without assigning the spectral interpretation to an arbitrary initial seed.

For the complete frozen phase-volume model, with its full ball instead of these cutoffs, the same image calculation in the reflection lesson gives −(2πh)−nγ(0,y)∫s2+ηTG(0,y)η≤1e2ids/h dη ds=−h−nWn(2d/h).(B46) \begin{gathered} -\frac{(2\pi h)^{-n}}{\gamma(0,y)} \int_{s^2+\eta^{\mathsf T}G(0,y)\eta\leq1} e^{2ids/h}\,d\eta\,ds\\ =-h^{-n}W_n(2d/h). \end{gathered} \tag{B46} The change θ=G(0,y)1/2η\theta=G(0,y)^{1/2}\eta has Jacobian dη=γ(0,y)dθd\eta=\gamma(0,y)d\theta; it cancels the density factor. Symmetry in ss turns the exponential into the cosine defining WnW_n. Removing the near-normal cutoff in the actual variable-coefficient problem is a separate estimate, not a consequence of this frozen identity.

10. An exact normal jump and boundary coupling

The preceding scalar transports also have an operator counterpart which fixes the normal source jump. We record it because an arbitrary choice of incident coefficients in (B37) is not yet a fundamental solution.

After the actual normal gauge already proved in Dirichlet commutators and a local diffraction estimate, localize to the same separated-root region, retain the energy E∈[E0,1]E\in[E_0,1] as a parameter, and extend its tangential symbol as in Sections 41–42 of Incoming phase neighborhoods for Dirichlet waves. The resulting bounded tangential family has normal expression Lh(E)=(hDa)2+Rh(a,E)L_h(E)=(hD_a)^2+R_h(a,E). It agrees with the gauged differential expression on the retained phase region, not globally. For any finite accuracy NN, the proved Riccati construction gives roots and their exact difference inverse: Rσ=Bσ2−ih∂aBσ+Rh,∥Rσ∥≤CNhN,∥Bσ−Bσ∗∥≤Ch,Ah=(B+−B−)−1,∥Ah∥≤C.(B47) \begin{gathered} \mathcal R_\sigma=B_\sigma^2-ih\partial_aB_\sigma+R_h,\\ \|\mathcal R_\sigma\|\leq C_Nh^N,\\ \|B_\sigma-B_\sigma^*\|\leq Ch,\\ A_h=(B_+-B_-)^{-1},\quad\|A_h\|\leq C. \end{gathered} \tag{B47} Norms are on tangential L2L^2. These statements hold after any fixed number of parameter derivatives, with the appropriate finite accuracy. Energy derivatives are ordinary compact-parameter derivatives in the same symbol recursion. The principal roots are ±E−r\pm\sqrt{E-r}; all actual lower terms are included in the finite roots.

For fixed h>0h>0, the bounded-operator integral equation constructs the evolution Uσ(a,b)U_\sigma(a,b) satisfying (hDa−Bσ(a))Uσ(a,b)=0,Uσ(b,b)=I,∥Uσ(a,b)∥≤eC∣a−b∣.(B48) \begin{gathered} (hD_a-B_\sigma(a))U_\sigma(a,b)=0,\\ U_\sigma(b,b)=I,\\ \|U_\sigma(a,b)\|\leq e^{C|a-b|}. \end{gathered} \tag{B48} For existence, successive substitution in the integral equation has its jj-th norm bounded by (Ch∣a−b∣)j/j!(C_h|a-b|)^j/j!; the series and its differentiated integral converge uniformly for each fixed hh. The same series proves uniqueness. The bound independent of hh is stronger than this existence estimate: apply the squared-norm identity and ∥Bσ−Bσ∗∥≤Ch\|B_\sigma-B_\sigma^*\|\leq Ch, exactly as in (T110), to each evolved vector, in either direction. Smooth parameter dependence follows by differentiating the integral equation; each fixed derivative has at worst a fixed power of h−1h^{-1}, because its inhomogeneous terms are bounded by the differentiated coefficient norms and the energy estimate. The group identity follows from uniqueness. In particular ∂bUσ(a,b)=−Uσ(a,b)(i/h)Bσ(b)\partial_bU_\sigma(a,b)=-U_\sigma(a,b)(i/h)B_\sigma(b), by differentiating that identity.

For an interior source distance 0<d<d00<d<d_0, put Mh(d)=(ih)−1Ah(d)M_h(d)=(ih)^{-1}A_h(d) and define Ghi(a,d)={U−(a,d)Mh(d),a≥d,U+(a,d)Mh(d),a≤d,Ghr(a,d)=−U−(a,0)U+(0,d)Mh(d),GhD=Ghi+Ghr.(B49) \begin{gathered} G_h^i(a,d)= \begin{cases} U_-(a,d)M_h(d),&a\geq d,\\ U_+(a,d)M_h(d),&a\leq d, \end{cases}\\ G_h^r(a,d)=-U_-(a,0)U_+(0,d)M_h(d),\\ G_h^D=G_h^i+G_h^r. \end{gathered} \tag{B49} This is an operator-valued distribution in the normal variable. The two incident values agree at a=da=d, and their ordinary derivative jump is [Ghi]a=d=0,[∂aGhi]a=d=ih(B−−B+)Mh=−h−2I.(B50) \begin{gathered} [G_h^i]_{a=d}=0,\\ [\partial_aG_h^i]_{a=d} =\frac ih(B_--B_+)M_h=-h^{-2}I. \end{gathered} \tag{B50} For a continuous piecewise smooth function the second distributional derivative is its piecewise second derivative plus this first-derivative jump times δ(a−d)\delta(a-d). This identity follows by integration by parts on the two intervals against a scalar test function, and also holds after pairing an operator with any two Hilbert-space vectors. Since (hDa)2=−h2∂a2(hD_a)^2=-h^2\partial_a^2, the singular term in LhGhDL_hG_h^D is exactly δ(a−d)I\delta(a-d)I; there is no derivative of a delta.

On each ordinary leg, LhUσ=RσUσL_hU_\sigma=\mathcal R_\sigma U_\sigma, by differentiating (B48) once more in the correct operator order. The reflected term has the same identity with R−\mathcal R_- at its target end. Equations (B47)–(B49) therefore give LhGhD=δ(a−d)I+Eh(a,d),GhD(0,d)=0,∥Eh(a,d)∥≤CNhN−1,∥Ghi(a,d)∥+∥Ghr(a,d)∥≤Ch−1.(B51) \begin{gathered} L_hG_h^D=\delta(a-d)I+\mathcal E_h(a,d),\\ G_h^D(0,d)=0,\qquad \|\mathcal E_h(a,d)\|\leq C_Nh^{N-1},\\ \|G_h^i(a,d)\|+\|G_h^r(a,d)\|\leq Ch^{-1}. \end{gathered} \tag{B51} The error bound is for the ordinary piecewise remainder; the singular term has already been identified exactly. The boundary value cancels because U−(0,0)=IU_-(0,0)=I. All constants are uniform as the interior source approaches the wall. On each open side of a=da=d, fixed parameter derivatives of the remainder lose only finitely many powers of hh; increasing the Riccati accuracy beforehand gives any prescribed differentiated error bound there. Across the source slice, derivatives in a,da,d are distributional and may also differentiate its step functions. Their delta coefficients are differences of the same arbitrarily small differentiated remainder values; no pointwise bound for a delta is asserted. No global resolvent bound at an eigenvalue has been assumed.

The normal source jump and Dirichlet cancellation in (B51) hold for the extended separated-root operator. Sections 22–27 compare its localized wave with the physical wave, including the extension and position-cutoff errors.

11. Phase action when the tangential frequency can be zero

Put m=n−1m=n-1. The normal roots in (B47) are bounded tangential operators of the form Bh=Op⁡h(bh)B_h=\operatorname{Op}_h(b_h), where bh=b0+hchb_h=b_0+h c_h, b0b_0 is real, and each symbol is a constant plus a smooth symbol supported in a fixed compact part of (z,ζ)(z,\zeta). All needed derivatives are bounded, uniformly in the compact energy and normal parameters. Derivatives in hh will not be required. The actual leading symbol on the retained region is b0=λσb_0=\lambda_\sigma.

We need phase action at η=0\eta=0, where the tangential phase gradient can vanish. The homogeneous formula in the scalar phase-action reading assumes a nonzero normalized phase gradient. Here a compact-frequency proof removes that assumption.

Let S(z,η)S(z,\eta) be a real smooth phase and let a(z,η;h)a(z,\eta;h) have fixed compact support in (z,η)(z,\eta), with uniform derivatives. All other variables are smooth compact parameters. Extend SS smoothly across the compact region needed below, with bounded derivatives there, and put F(z,w,η)=∫01Sz(z+vw,η) dv,S(z+w,η)−S(z,η)=w⋅F(z,w,η).(B52) \begin{gathered} F(z,w,\eta)=\int_0^1 S_z(z+vw,\eta)\,dv,\\ S(z+w,\eta)-S(z,\eta)=w\cdot F(z,w,\eta). \end{gathered} \tag{B52} For each positive integer JJ, direct insertion of the left-quantized kernel gives BSa=e−iS/hBh(eiS/ha),BSa=∑∣α∣<J(h/i)∣α∣α!Cα+hJrJ,Cα=(∂wα∂ραG)(0,0),G(w,ρ)=bh(z,ρ+F(z,w,η))⋅a(z+w,η;h).(B53) \begin{gathered} \mathcal B_Sa=e^{-iS/h}B_h(e^{iS/h}a),\\ \mathcal B_Sa=\sum_{|\alpha|<J}\frac{(h/i)^{|\alpha|}}{\alpha!} C_\alpha+h^Jr_J,\\ C_\alpha=(\partial_w^\alpha\partial_\rho^\alpha G)(0,0),\\ G(w,\rho)=b_h(z,\rho+F(z,w,\eta))\\ \qquad\cdot a(z+w,\eta;h). \end{gathered} \tag{B53} Every fixed derivative of rJr_J in z,ηz,\eta and the compact parameters is bounded. Its η\eta-support stays in the fixed support of the amplitude, and its zz-support stays in a fixed compact set. No lower bound for ∣Sz∣|S_z| appears.

To prove this, separate the constant part of bhb_h; its action is exactly that constant times aa, with zero positive-order coefficients. For the compact part the conjugated integral has phase S(z+w,η)−S(z,η)−wζS(z+w,\eta)-S(z,\eta)-w\zeta. The change ρ=ζ−F(z,w,η)\rho=\zeta-F(z,w,\eta) has Jacobian one and makes this phase exactly −wρ-w\rho. Its amplitude is smooth and compact in (w,ρ)(w,\rho), uniformly in all retained parameters: zz is in the compact base support of the symbol, z+wz+w in that of aa, and ζ\zeta in the compact frequency support of the symbol. The quadratic stationary-phase proof (P4)–(P8) in Phase geometry and stationary phase, applied with parameter h−1h^{-1}, has Hessian (0−I−I0)\left(\begin{smallmatrix}0&-I\\-I&0\end{smallmatrix}\right). Its determinant has absolute value one and its signature is zero. Its factor (2πh)m(2\pi h)^m cancels the quantization prefactor; its differential operator is −2∂w⋅∂ρ-2\partial_w\cdot\partial_\rho. These facts give precisely (B53), including its differentiated finite remainder. Outside the union of the two compact base supports the action and every term vanish. If the amplitude vanishes for a parameter frequency η\eta, the action does too. This proves the support and parameter assertions for the actual remainder, not just its formal coefficients.

In particular the first two terms, with bh=b0+hchb_h=b_0+h c_h, are BSa=b0a+hcha+hi∑j(b0)ζj∂ja+h2i∑j,k(b0)ζjζkSjka+O(h2).(B54) \begin{aligned} \mathcal B_Sa={}&b_0a+h c_ha\\ &+\frac hi\sum_j(b_0)_{\zeta_j}\partial_ja\\ &+\frac h{2i}\sum_{j,k}(b_0)_{\zeta_j\zeta_k}S_{jk}a\\ &+O(h^2). \end{aligned} \tag{B54} All symbol factors and their frequency derivatives in (B54) are evaluated at (z,Sz)(z,S_z). The remainder has the same smooth parameter meaning as (B53), after the critical exponential has been removed. This formula is valid at the normal ray itself.

12. Norms that turn an operator error into a kernel error

For an integer s≥0s\geq0, use the semiclassical Sobolev norm with Fourier weight ⟨hξ⟩s\langle h\xi\rangle^s, denoted Hhs(Rm)H_h^s(\mathbb R^m); negative orders are its dual norms. For positive integers this norm is uniformly equivalent to the sum of ∥(hD)αu∥2\|(hD)^\alpha u\|_2, ∣α∣≤s|\alpha|\leq s, by comparison of the corresponding polynomials in Fourier space. The Fourier normalization and dual pairing are those of the Fourier reading.

The exact normal evolutions and difference inverse from (B47)–(B48) obey ∥Uσ(a,b)∥Hh±s→Hh±s≤Cs,∥Ah(a)∥Hh±s→Hh±s≤Cs.(B55) \begin{gathered} \|U_\sigma(a,b)\|_{H_h^{\pm s}\to H_h^{\pm s}} \leq C_s,\\ \|A_h(a)\|_{H_h^{\pm s}\to H_h^{\pm s}} \leq C_s. \end{gathered} \tag{B55} The first estimate has an energy proof, not an exponential bound of size eC/he^{C/h}. The exact identity [hDj,Op⁡h(bh)]=−ihOp⁡h(∂zjbh)(B56) [hD_j,\operatorname{Op}_h(b_h)] =-ih\operatorname{Op}_h(\partial_{z_j}b_h) \tag{B56} follows by differentiating the kernel and integrating the input derivative by parts. The finite-derivative operator bound (N17) bounds each coefficient uniformly. Iterating (B56) expresses [(hD)α,Bh]u[(hD)^\alpha,B_h]u as terms of norm at most Csh∥u∥HhsC_sh\|u\|_{H_h^s}. Apply the squared-norm argument of (B48) to every (hD)αu(hD)^\alpha u, retain these commutators divided by hh, sum and integrate. This proves the first bound for smooth inputs. Existence in HhsH_h^s also follows first from the bounded-operator integral equation there, since (B56) makes BhB_h bounded on that space for each fixed hh; uniqueness identifies it with the L2L^2 evolution. Density extends the uniform energy estimate. The adjoint evolution with reversed normal endpoints has the same skew-part and commutator bounds, giving the negative-order statement by duality.

For the inverse, write B+−B−=2k0I+KhB_+-B_-=2k_0I+K_h, with k0>0k_0>0 constant and KhK_h a compact-frequency operator. Differentiating its kernel shows Kh:L2→HhsK_h:L^2\to H_h^s bounded uniformly: every output hDhD produces either a bounded frequency factor or hh times a symbol derivative, and (N17) applies. If u∈Hhsu\in H_h^s and v=Ahuv=A_hu, its already established L2L^2 identity gives v=(2k0)−1(u−Khv)v=(2k_0)^{-1}(u-K_hv). This first proves v∈Hhsv\in H_h^s, then bounds that norm using the L2L^2 inverse bound. The adjoint compact-frequency kernel has the same output-derivative estimate, so the same argument and duality prove the negative-order bound. Parameter differentiation of the inverse identity preserves these bounds. Differentiating the evolution equation or its integral formula costs at most a finite power of h−1h^{-1} for each fixed number of parameter derivatives, by the same inhomogeneous energy estimate.

There is a direct quantitative kernel consequence. If Rh:Hh−s→HhsR_h:H_h^{-s}\to H_h^s, and s>m/2+js>m/2+j, Fourier integration gives the following bounds for ∣α∣,∣β∣≤j|\alpha|,|\beta|\leq j: ∥∂yβδy∥Hh−s≤Cs,βh−m/2−∣β∣,∣∂zα∂yβKRh(z,y)∣≤Ch−m−∣α∣−∣β∣∥Rh∥Hh−s→Hhs.(B57) \begin{gathered} \|\partial_y^\beta\delta_y\|_{H_h^{-s}} \leq C_{s,\beta}h^{-m/2-|\beta|},\\ |\partial_z^\alpha\partial_y^\beta K_{R_h}(z,y)|\\ \leq C h^{-m-|\alpha|-|\beta|} \|R_h\|_{H_h^{-s}\to H_h^s}. \end{gathered} \tag{B57} For the first bound, substitute θ=hξ\theta=h\xi in the squared Fourier norm of the differentiated delta. The remaining integral of ∣θ∣2∣β∣⟨θ⟩−2s|\theta|^{2|\beta|}\langle\theta\rangle^{-2s} is finite. The same estimate is the norm of derivative evaluation on HhsH_h^s. Pair that evaluation with Rh∂yβδyR_h\partial_y^\beta\delta_y to obtain the second bound. Taking ss slightly larger, dominated convergence of these Fourier integrals proves continuous differentiability in z,yz,y; integration against compact smooth inputs identifies this function with the distribution kernel. Thus arbitrary finite weighted Sobolev accuracy implies arbitrary finite ordinary kernel accuracy, with the displayed powers of hh retained.

We will also use a finite local symbol for AhQhA_hQ_h, where Qh=Op⁡h(q)Q_h=\operatorname{Op}_h(q) is a smooth compact phase cutoff. For any chosen accuracy and any fixed ss, AhQh=Op⁡h(qA,h)+RA,h,qA,h(z,η)=q(z,η)2E−r(a,z,η)+hq1,h(z,η),∥RA,h∥Hh−s→Hhs=O(hN).(B58) \begin{gathered} A_hQ_h=\operatorname{Op}_h(q_{A,h})+R_{A,h},\\ q_{A,h}(z,\eta)=\frac{q(z,\eta)}{2\sqrt{E-r(a,z,\eta)}}\\ \qquad+h q_{1,h}(z,\eta),\\ \|R_{A,h}\|_{H_h^{-s}\to H_h^s}=O(h^N). \end{gathered} \tag{B58} Here and below an arbitrary prescribed NN is obtained by choosing a sufficiently long finite expansion; the constants may depend on that choice. All symbol derivatives are bounded, and qA,hq_{A,h} has fixed compact support inside the retained phase region after allowing fixed margins. The finite inverse recursion of (T104) starts with (2E−r)−1(2\sqrt{E-r})^{-1} and cancels the actual left product residual successively. Its symbols are a constant plus compact terms. The exact product formula (N19) and its Taylor remainder (N20) show that the inverse residual is hNOp⁡h(rN)h^N\operatorname{Op}_h(r_N), with all derivatives bounded and compact frequency support: expand products into their constant and compact parts and apply (N19) to each compact right factor. Constant right factors leave the compact left symbol itself. Such remainders map Hh−sH_h^{-s} to HhsH_h^s uniformly after removal of hNh^N. Indeed right multiplication by the Fourier weight is exact multiplication of the left symbol by ⟨η⟩s\langle\eta\rangle^s; output hDhD derivatives again give bounded compact-frequency symbols. Multiplication by the exact inverse, using (B55), proves the claimed error for the finite inverse. A further application of (N19)–(N20) to its product with QhQ_h proves (B58). Parameter derivatives are included by increasing the finite accuracy. This argument does not give actual operator remainders the supports of formal coefficients.

13. A phase kernel for the exact normal evolution

Choose a compact initial phase patch whose two normal flows stay in the region of (B25) for all retained normal endpoints. Let qhq_h be a symbol supported in this patch with uniformly bounded derivatives. It may depend on hh and on the compact parameters. Write Φσ(a,z;b,η,E)\Phi_\sigma(a,z;b,\eta,E) for the phase constructed in Section 6 with initial value z⋅ηz\cdot\eta at a=ba=b. Thus Sσi(a,z;b,y,η,E)=Φσ−y⋅ηS^i_\sigma(a,z;b,y,\eta,E)=\Phi_\sigma-y\cdot\eta, and Φzη=I+O(∣a−b∣)\Phi_{z\eta}=I+O(|a-b|) is uniformly invertible on a sufficiently short fixed collar.

For every requested finite kernel accuracy, construct Vσ(a,b)f(z)=(2πh)−m∬ei(Φσ−yη)/hvσf(y) dη dy,Vσ(b,b)=Op⁡h(qh).(B59) \begin{gathered} V_\sigma(a,b)f(z)\\ =(2\pi h)^{-m}\iint e^{i(\Phi_\sigma-y\eta)/h} v_\sigma f(y)\,d\eta\,dy,\\ V_\sigma(b,b)=\operatorname{Op}_h(q_h). \end{gathered} \tag{B59} In (B59), the suppressed arguments are Φσ=Φσ(a,z;b,η,E)\Phi_\sigma=\Phi_\sigma(a,z;b,\eta,E) and vσ=vσ(a,z;b,η,E,h)v_\sigma=v_\sigma(a,z;b,\eta,E,h). The amplitude is smooth, has fixed compact support in its phase patch, and has uniform derivatives in all displayed variables except that no hh-derivatives are asserted. It is a finite sum of powers of hh with bounded smooth coefficients, allowed to depend uniformly on hh.

For clarity the first transport equation follows from (B54), with Bσ=Op⁡h(λσ+hcσ,h)B_\sigma=\operatorname{Op}_h(\lambda_\sigma+h c_{\sigma,h}). Its order-hh operator is Tσ,hv=1i(∂a−λσ,ζ⋅∂z)v−cσ,h(a,z,Φz,E)v−12i∑j,kλσ,ζjζk(a,z,Φz,E)Φzjzkv.(B60) \begin{aligned} \mathscr T_{\sigma,h}v={}&\frac1i (\partial_a-\lambda_{\sigma,\zeta}\cdot\partial_z)v\\ &-c_{\sigma,h}(a,z,\Phi_z,E)v\\ &-\frac1{2i}\sum_{j,k} \lambda_{\sigma,\zeta_j\zeta_k}(a,z,\Phi_z,E) \Phi_{z_jz_k}v. \end{aligned} \tag{B60} All coefficients here are evaluated on the phase, and the leading order vanishes by Φa=λσ(a,z,Φz,E)\Phi_a=\lambda_\sigma(a,z,\Phi_z,E). Set the leading amplitude's initial value equal to qhq_h, and solve Tσ,hv0=0\mathscr T_{\sigma,h}v_0=0. At each subsequent order, solve the same inhomogeneous scalar transport equation with the negative of the actual remaining coefficient from (B53), and with zero initial value. The integrating-factor proof in Section 8 applies because its base vector field is the same smooth characteristic flow. It gives every uniform parameter derivative. All coefficients remain supported in the transported initial support: finite differential operators do not enlarge support, and their inhomogeneous transport has zero initial value. The phase can be smoothly extended beyond a slightly larger patch; the amplitudes vanish wherever that extension need not satisfy the eikonal equation. The actual off-support action errors are covered by the remainder in (B53).

Here are operator, not just formal, error bounds for this construction. After cancellation through order hJh^J, its first-order residual kernel has the form hJ+1(2πh)−m∫ei(Φ−yη)/hrJ dηh^{J+1}(2\pi h)^{-m}\int e^{i(\Phi-y\eta)/h}r_J\,d\eta, with all relevant amplitude derivatives bounded and compact (z,η)(z,\eta)-support. For bounded yy, its absolute value is at most ChJ+1−mC h^{J+1-m}. For large ∣y∣|y|, the phase derivative Φη−y\Phi_\eta-y is bounded below by a constant times 1+∣y∣1+|y|. Repeated integration by parts in η\eta gives any desired integrable decay in yy, with additional factors of hh. The same bounds hold after any fixed output and input semiclassical derivatives hDz,hDyhD_z,hD_y, since they produce bounded phase derivatives and bounded amplitude derivatives. Schur's integral inequality therefore gives, for every fixed even integer s≥0s\geq0, ∥(hDa−Bσ)Vσ∥Hh−s→Hhs≤CJ,shJ+1−m.(B61) \|(hD_a-B_\sigma)V_\sigma\|_{H_h^{-s}\to H_h^s} \leq C_{J,s}h^{J+1-m}. \tag{B61} One can verify this norm assertion directly by writing a negative-order input as (1−h2Δy)s/2f(1-h^2\Delta_y)^{s/2}f with f∈L2f\in L^2, integrating those finitely many derivatives onto the kernel, and then applying output derivatives and Schur. The even integer restriction is sufficient for every desired kernel derivative in (B57). Schur's inequality itself is the two weighted Cauchy–Schwarz integrations in the finite-derivative operator proof; it requires both integrable kernel bounds, supplied here by compact zz-support and the preceding yy-decay.

The initial identity in (B59) is exact, because every positive-order transport correction starts at zero. Variation of constants for the actual evolution, using (B55), now gives Eσ(a,b)=Uσ(a,b)Op⁡h(qh)−Vσ(a,b),Fσ(v,b)=(hDv−Bσ(v))Vσ(v,b),Eσ(a,b)=−ih∫baUσ(a,v)Fσ(v,b) dv,∥Eσ(a,b)∥Hh−s→Hhs≤ChJ−m.(B62) \begin{gathered} \mathcal E_\sigma(a,b) =U_\sigma(a,b)\operatorname{Op}_h(q_h)-V_\sigma(a,b),\\ \mathcal F_\sigma(v,b) =(hD_v-B_\sigma(v))V_\sigma(v,b),\\ \mathcal E_\sigma(a,b) =-\frac ih\int_b^a U_\sigma(a,v)\mathcal F_\sigma(v,b)\,dv,\\ \|\mathcal E_\sigma(a,b)\|_{H_h^{-s}\to H_h^s} \leq C h^{J-m}. \end{gathered} \tag{B62} The sign follows by differentiating the right side; the oriented integral handles either ordering of the endpoints. In particular the forcing loses one power of hh, which has been retained. Differentiate this actual integral identity to obtain normal-endpoint and energy derivatives. The differentiated evolution contributes only fixed powers of h−1h^{-1}, as proved after (B55); differentiated residual phases contribute one such power per ordinary parameter derivative. Endpoint terms are the same residuals or their derivatives at an endpoint. There are finitely many terms for any prescribed derivative order, so increasing JJ gives arbitrary accuracy for them as well.

Finally apply (B57), with an even ss larger than all desired derivative orders. We have proved that, for any fixed finite collection of derivatives and any prescribed NN, [Uσ(a,b)Op⁡h(qh)](z,y)=[Vσ(a,b)](z,y)+Rh,∣∂αRh∣≤CN,αhN.(B63) \begin{gathered} [U_\sigma(a,b)\operatorname{Op}_h(q_h)](z,y)\\ =[V_\sigma(a,b)](z,y)+R_h,\\ |\partial^\alpha R_h|\leq C_{N,\alpha}h^N. \end{gathered} \tag{B63} The estimates include both normal endpoints through zero and through equality, and the compact energy parameter. This identifies a finite phase kernel for the exact normal operator; it is stronger than a wavefront assertion. Zero tangential frequency has not been removed.

14. The reflected normal operator and its source coefficient

Let Qh(d,E)=Op⁡h(q(d,z,η,E))Q_h(d,E)=\operatorname{Op}_h(q(d,z,\eta,E)), with smooth bounded compact support as above, and define the two normalized reflected operators Hσ,h(a,d;E)=−Uσ(a,0;E)U−σ(0,d;E)⋅Ah(d,E)Qh(d,E).(B64) \begin{gathered} H_{\sigma,h}(a,d;E)\\ =-U_\sigma(a,0;E)U_{-\sigma}(0,d;E)\\ \qquad\cdot A_h(d,E)Q_h(d,E). \end{gathered} \tag{B64} For σ=−1\sigma=-1, this is exactly ihGhrQhihG_h^rQ_h from (B49). The other orientation has the same source-jump construction after interchanging the roots and reversing the sign of its initial jump factor. More explicitly its incident factor is −σ(ih)−1Ah-\sigma(ih)^{-1}A_h, so its reflected part satisfies (−σih)Gσ,hrQh=Hσ,h(-\sigma ih)G^r_{\sigma,h}Q_h=H_{\sigma,h}. Substitution in (B50) proves that both unnormalized Green families have the source δ(a−d)I\delta(a-d)I; after the right cutoff this source is δ(a−d)Qh\delta(a-d)Q_h.

For every finite requested kernel accuracy, these exact operators have the representation Hσ,h(a,d;E)(z,y)=(2πh)−m∫eiSσr/hcσ dη+Rσ,h,∣∂αRσ,h∣≤CN,αhN.(B65) \begin{gathered} H_{\sigma,h}(a,d;E)(z,y)\\ =(2\pi h)^{-m}\int e^{iS^r_\sigma/h} c_\sigma\,d\eta+R_{\sigma,h},\\ |\partial^\alpha R_{\sigma,h}|\leq C_{N,\alpha}h^N. \end{gathered} \tag{B65} In (B65), Sσr=Sσr(a,z;d,y,η,E)S^r_\sigma=S^r_\sigma(a,z;d,y,\eta,E) and cσ=cσ(a,z;d,η,E,h)c_\sigma=c_\sigma(a,z;d,\eta,E,h). All derivatives of the compactly supported amplitude cσc_\sigma in its ordinary parameters are uniformly bounded. At the common zero normal slice it obeys cσ(0,z;0,η,E,h)=−q(0,z,η,E)2E−r(0,z,η)+hrσ,h(z,η,E).(B66) \begin{gathered} c_\sigma(0,z;0,\eta,E,h)\\ =-\frac{q(0,z,\eta,E)}{2\sqrt{E-r(0,z,\eta)}} +h r_{\sigma,h}(z,\eta,E). \end{gathered} \tag{B66} where rσ,hr_{\sigma,h} and all required derivatives are bounded. Thus the leading frozen coefficient is fixed by the exact inverse difference and source jump, rather than chosen as independent data.

To prove these assertions without assuming a composition theorem at zero distance, first use (B58) for AhQhA_hQ_h. Apply the single-leg construction of Section 13 to U−σ(a,d)Op⁡h(qA,h)U_{-\sigma}(a,d)\operatorname{Op}_h(q_{A,h}) and restrict its target normal variable to zero. The phase is S−σi(0,z;d,y,η,E)S^i_{-\sigma}(0,z;d,y,\eta,E); its amplitude has all the uniform source-distance and energy derivatives just proved. Start a new phase transport on the σ\sigma leg at a=0a=0, with the negative of this incident amplitude as initial value. Its phase is exactly SσrS^r_\sigma by (B26). The same compact phase-action expansion and scalar recursion work for this initial phase: its mixed derivative in (z,η)(z,\eta) is still I+O(d)I+O(d), and its phase and amplitude derivatives are uniformly bounded. Its initial kernel is the negative of the incident approximate kernel exactly, not merely to leading order.

Apply the inhomogeneous estimate (B62) to this second leg. The errors in the initial incident kernel and in (B58) are propagated by the bounded operators (B55); the new forcing has the bounds (B61). Parameter derivatives lose only fixed powers as before. Equation (B57) turns the resulting weighted Sobolev error into (B65). This proof does not multiply two oscillatory integrals and assume their remainders retain compact supports. At a=d=0a=d=0, both phase transports have length zero, all their correction integrals vanish, and the chosen amplitude is exactly −qA,h-q_{A,h}. Its expansion (B58) proves (B66).

15. Uniform freezing for the exact normal family

Let χ(E)\chi(E) be smooth on the energy interval and zero near E0E_0. Define a quantity from the exact normal operators, with diagonal density relative to dVgdV_g, by Nhr(d,y)=12πh γ(d,y)∑σ=±1∫E01χ(E)⋅Hσ,h(d,d;E)(y,y) dE.(B67) \begin{gathered} \mathcal N_h^r(d,y)\\ =\frac{1}{2\pi h\,\gamma(d,y)} \sum_{\sigma=\pm1}\int_{E_0}^1\chi(E)\\ \qquad\cdot H_{\sigma,h}(d,d;E)(y,y)\,dE. \end{gathered} \tag{B67} The symbol Nhr\mathcal N_h^r denotes this normal-operator quantity, not the spectral counting function or the actual spectral projector. Equations (B65)–(B66) and the now verified metric-phase hypotheses imply Nhr(d,y)−Nh,0r(d,y)=O(h1−n),Nh,0r(d,y)=−(2πh)−nγ(0,y)⋅∑σ∫E01∫e2iσdλ0/h⋅χ(E)q(0,y,η,E)2λ0 dη dE,λ0=E−r(0,y,η).(B68) \begin{gathered} \mathcal N_h^r(d,y)-\mathcal N_{h,0}^r(d,y)=O(h^{1-n}),\\ \mathcal N_{h,0}^r(d,y) =-\frac{(2\pi h)^{-n}}{\gamma(0,y)}\\ \quad\cdot\sum_\sigma\int_{E_0}^1\int e^{2i\sigma d\lambda_0/h}\\ \qquad\cdot\frac{\chi(E)q(0,y,\eta,E)}{2\lambda_0} \,d\eta\,dE,\\ \lambda_0=\sqrt{E-r(0,y,\eta)}. \end{gathered} \tag{B68} The error is uniform for 0≤d≤d00\leq d\leq d_0 and all retained yy. Indeed, insert (B65) with arbitrary kernel accuracy, so its energy integral contributes O(hN−1)O(h^{N-1}). The remaining prefactors multiply to (2πh)−n(2\pi h)^{-n}, because m=n−1m=n-1. On the diagonal the phase is dψσd\psi_\sigma. The amplitude χ(E)γ(d,y)−1cσ(d,y;d,η,E,h)\chi(E)\gamma(d,y)^{-1}c_\sigma(d,y;d,\eta,E,h) has uniform distance and energy derivatives and vanishes near E0E_0. Apply Lemma 5.1 with hh as an additional uniformly bounded-amplitude parameter. Equations (B29)–(B33) verify all phase hypotheses. This replaces its smooth distance arguments by zero with error O(h1−n)O(h^{1-n}). At zero, (B66) fixes the leading coefficient in (B68); the remaining amplitude has an explicit factor hh, so its absolute integral is also O(h1−n)O(h^{1-n}). Choose the initial kernel accuracy large enough to absorb its tail. This proves (B68) for the exact normal evolution and inverse operators, including the wall limit.

The multiplicative normal gauge used in (B47) does not alter this diagonal normalization on the retained region. If P~=κPκ−1\widetilde P=\kappa P\kappa^{-1}, restoring a kernel multiplies its coordinate coefficient by κ(a,z)−1κ(d,y)\kappa(a,z)^{-1}\kappa(d,y). On the diagonal this factor is exactly one. Its off-diagonal derivatives are bounded on the compact collar and therefore preserve every finite remainder estimate above. The volume factor γ−1\gamma^{-1} remains exactly the one proved in (B41).

The normalization and error in (B68) concern the exact normal family. Sections 18–27 supply the physical-time normalization and the quantitative comparison with the actual near-normal spectral contribution.

16. An extension compatible with physical time

The small residual in (B51) is sufficient for the reflected estimates already proved. It is not an exact wave equation: normal differentiation across its incident source slice can produce small delta terms. We now remove that residual. We also choose the extension so that its energy dependence is exactly subtraction of EE; otherwise a temporal Fourier inversion need not yield a second-order equation in physical time.

All preceding root and transport arguments work on any compact positive energy interval. Choose J=[E∗,E∗]J=[E_*,E^*], with 0<E∗<E0<1<E∗0<E_*<E_0<1<E^*, and reduce the retained tangential ball if necessary. Extend the actual tangential cometric smoothly across a larger compact chart. Choose a smooth phase cutoff equal to one on both retained flow tubes, supported where r≤E∗/2r\leq E_*/2, and between zero and one. Multiplying rr by this cutoff gives a real smooth compact symbol rer_e, with 0≤re≤E∗/20\leq r_e\leq E_*/2. Extend every actual gauged lower-order tangential coefficient with a cutoff equal to one on the same tubes. Its left symbol has the form hρ1(a,z,ζ;h)h\rho_1(a,z,\zeta;h), with bounded derivatives and compact phase support. Thus we may and do use Th(a)=Op⁡h(re+hρ1),Rh(a,E)=Th(a)−EI,Lh(E)=(hDa)2+Th(a)−EI.(B69) \begin{gathered} T_h(a)=\operatorname{Op}_h(r_e+h\rho_1),\\ R_h(a,E)=T_h(a)-EI,\\ L_h(E)=(hD_a)^2+T_h(a)-EI. \end{gathered} \tag{B69} Here ThT_h is independent of EE. The leading roots are σE−re\sigma\sqrt{E-r_e}, equal to σE\sigma\sqrt E outside a compact phase set. Their gap has a uniform positive lower bound. The proofs in Sections 10–15 apply verbatim with the exterior constant k0=Ek_0=\sqrt E; its energy derivatives are bounded on JJ. On the retained tubes the expression still includes all actual gauged lower terms. The choice (B69) is a particular admissible extension, not an assertion that it equals the actual differential operator everywhere.

The finite Riccati residual can be estimated more strongly than in (B47). Given a finite accuracy LL, it is a finite sum of hLh^L times bounded symbols with fixed compact frequency support. This follows from the exact product formula (N19), as in the inverse proof (B58): the constant terms cancel, and every other product has a compact factor; constant right factors leave the compact left factor. Consequently, for every fixed integer s≥0s\geq0 and any fixed number of ordinary parameters derivatives, ∥∂αRσ∥Hh−s→Hhs≤CL,s,αhL.(B70) \|\partial^\alpha\mathcal R_\sigma\| _{H_h^{-s}\to H_h^s}\leq C_{L,s,\alpha}h^L. \tag{B70} Choose the finite recursion long enough for the stated LL. The compact-frequency smoothing proof following (B58) proves (B70), including normal and energy derivatives. There is no assertion about differentiation in hh.

For a pair (w,v)(w,v), put da=hDad_a=hD_a and use the invertible change w=V++V−,v=B+V++B−V−,V+=Ah(v−B−w),V−=w−V+.(B71) \begin{gathered} w=V_++V_-,\qquad v=B_+V_++B_-V_-,\\ V_+=A_h(v-B_-w),\qquad V_-=w-V_+. \end{gathered} \tag{B71} The change and its inverse are uniformly bounded on Hh±s⊕Hh±sH_h^{\pm s}\oplus H_h^{\pm s}, by (B55), the commutator proof there for the roots, and the same bounds for their parameter derivatives. The exact equation Lh(E)w=FL_h(E)w=F, with v=dawv=d_aw, becomes F~=F−R+V+−R−V−,(da−B+)V+=AhF~,(da−B−)V−=−AhF~.(B72) \begin{gathered} \widetilde F=F-\mathcal R_+V_+-\mathcal R_-V_-,\\ (d_a-B_+)V_+=A_h\widetilde F,\\ (d_a-B_-)V_-=-A_h\widetilde F. \end{gathered} \tag{B72} This is the direct differentiation used in (T107); it preserves every operator order. In particular its coupling has norm O(hL)O(h^L) on each of these spaces. One way to verify existence and the uniform bound is to apply variation of constants with the block diagonal evolution diag⁡(U+,U−)\operatorname{diag}(U_+,U_-). The successive iterates of the coupling integral have norm at most C(ChL−1∣a−b∣)j/j!C(C h^{L-1}|a-b|)^j/j!. The series converges, is unique by the same estimate for a difference, and is bounded uniformly for L≥1L\geq1 on the fixed collar. With forcing it gives ∥(w,daw)(a)∥Hh±s⊕Hh±s≤Cs∥(w,daw)(b)∥Hh±s⊕Hh±s+Csh∫[a,b]∥F(v)∥Hh±s ∣dv∣.(B73) \begin{gathered} \|(w,d_aw)(a)\|_{H_h^{\pm s}\oplus H_h^{\pm s}}\\ \leq C_s\|(w,d_aw)(b)\|_{H_h^{\pm s}\oplus H_h^{\pm s}}\\ \quad+\frac{C_s}{h}\int_{[a,b]}\|F(v)\|_{H_h^{\pm s}}\,|dv|. \end{gathered} \tag{B73} For the forcing term use the uniform boundedness of AhA_h and sum the same iterates; either ordering of the endpoints is allowed. This proves stability for the exact second-order equation, without an exponential of order eC/he^{C/h}. Ordinary parameter derivatives of its integral identity lose at most finitely many powers of h−1h^{-1}. To see this explicitly, each normal derivative uses da(w,v)=(v,−Rhw+F)d_a(w,v)=(v,-R_hw+F); each energy or initial-slice derivative differentiates a bounded coefficient, initial datum or forcing and then uses (B73). Induction gives a finite loss for each fixed number of derivatives.

17. Exact normal Green families

Let Fσ(a,b;E)F_\sigma(a,b;E) be the first component of the exact second-order solution with data w(b)=Iw(b)=I, daw(b)=Bσ(b)d_aw(b)=B_\sigma(b). It satisfies Lh(E)Fσ(a,b;E)=0,Fσ(b,b;E)=I,daFσ(b,b;E)=Bσ(b),∥Fσ−Uσ∥Hh−s→Hhs≤CshL−1.(B74) \begin{gathered} L_h(E)F_\sigma(a,b;E)=0,\\ F_\sigma(b,b;E)=I,\qquad d_aF_\sigma(b,b;E)=B_\sigma(b),\\ \|F_\sigma-U_\sigma\|_{H_h^{-s}\to H_h^s} \leq C_s h^{L-1}. \end{gathered} \tag{B74} Indeed their difference has zero value and zero first normal datum at a=ba=b, and forcing −RσUσ-\mathcal R_\sigma U_\sigma. Use (B70), the negative-order bound for UσU_\sigma, and (B73) with output HhsH_h^s. This also bounds its first semiclassical normal derivative. Differentiating this identity proves every fixed endpoint and energy derivative with a finite further power loss. Thus, by increasing LL, all these differences have any prescribed finite ordinary kernel accuracy, by (B57). This is a quantitative comparison with an exact solution, not a formal factorization.

For either σ=±1\sigma=\pm1, define Mσ(d)=−σ(ih)−1Ah(d)M_\sigma(d)=-\sigma(ih)^{-1}A_h(d) and, for an interior source 0<d<d00<d<d_0, set G^σi(a,d)={Fσ(a,d)Mσ(d),a≥d,F−σ(a,d)Mσ(d),a≤d,G^σr(a,d)=−Fσ(a,0)F−σ(0,d)Mσ(d),G^σD=G^σi+G^σr.(B75) \begin{gathered} \widehat G^i_\sigma(a,d)= \begin{cases} F_\sigma(a,d)M_\sigma(d),&a\geq d,\\ F_{-\sigma}(a,d)M_\sigma(d),&a\leq d, \end{cases}\\ \widehat G^r_\sigma(a,d) =-F_\sigma(a,0)F_{-\sigma}(0,d)M_\sigma(d),\\ \widehat G^D_\sigma=\widehat G^i_\sigma+\widehat G^r_\sigma. \end{gathered} \tag{B75} The two incident values agree at the source. Their derivative jump is (i/h)(Bσ−B−σ)Mσ=−h−2I(i/h)(B_\sigma-B_{-\sigma})M_\sigma=-h^{-2}I, since Bσ−B−σ=σ(B+−B−)B_\sigma-B_{-\sigma}=\sigma(B_+-B_-). Every ordinary leg solves the exact second-order equation. The integration-by-parts jump proof of (B50) now gives the exact identities Lh(E)G^σD=δ(a−d)I,G^σD(0,d)=0,Lh(E)(G^−D−G^+D)=0.(B76) \begin{gathered} L_h(E)\widehat G^D_\sigma=\delta(a-d)I,\\ \widehat G^D_\sigma(0,d)=0,\\ L_h(E)(\widehat G^D_- -\widehat G^D_+)=0. \end{gathered} \tag{B76} No ordinary residual remains. Moreover the difference in the last line is smooth across a=da=d: its value jump and first-derivative jump both vanish. On the two sides it solves the same smooth bounded-operator Cauchy equation. Uniqueness identifies both sides with the solution from their common Cauchy data at a=da=d. Those data depend smoothly on d,Ed,E, so the difference is smooth jointly in both normal variables and energy. This justifies all higher derivatives without assigning a pointwise bound to a delta. Individual incident families still have their required first-derivative jump. At d=0d=0 only the uniform limiting estimates are asserted, not an interior delta source on the boundary.

For the same retained right cutoff Qh(d,E)Q_h(d,E), put H^σ,h=−Fσ(a,0)F−σ(0,d)Ah(d)Qh(d,E),H^σ,h=(−σih)G^σrQh,∂α(H^σ,h−Hσ,h)(z,y)=O(hN).(B77) \begin{gathered} \widehat H_{\sigma,h} =-F_\sigma(a,0)F_{-\sigma}(0,d)A_h(d)Q_h(d,E),\\ \widehat H_{\sigma,h} =(-\sigma ih)\widehat G^r_\sigma Q_h,\\ \partial^\alpha(\widehat H_{\sigma,h}-H_{\sigma,h})(z,y) =O(h^N). \end{gathered} \tag{B77} For any prescribed N,αN,\alpha, choose LL large first. Subtract the two ordered products, replacing one factor at a time. Equation (B74) supplies arbitrary weighted smoothing accuracy for the difference factor; all remaining factors are bounded on both weighted spaces. The inverse and cutoff obey (B55) and (B58). The same argument after differentiation and (B57) proves the last line. It also applies to either ordinary incident leg. Hence (B65)–(B68), including the leading coefficient and uniform frozen estimate, hold for these exact second-order reflected families as well. We have removed the equation residual without altering the finite leading coefficient or the earlier estimate.

18. Temporal orientation and the exact source prefactor

Take temporal frequencies with τ2∈J\tau^2\in J, separated from zero, and set E=τ2E=\tau^2. Choose σ=−sgn⁡τ\sigma=-\operatorname{sgn}\tau for the outgoing incident leg a≥da\geq d and for the reflected leg; the incident leg a≤da\leq d has the opposite root. This orientation has a precise travel-time inequality.

Differentiate the action (B27) in τ\tau at fixed target position. Its endpoint variations cancel by the same variational identity that proved (B28). Along an incident characteristic this leaves the integral of ∂τλσ=στ/τ2−r\partial_\tau\lambda_\sigma=\sigma\tau/\sqrt{\tau^2-r}. On the two reflected legs the intermediate endpoint variations cancel against each other, since their phase gradients match at the wall. Therefore ∂τSσi=∫daσττ2−r(v,Z,Ξ) dv,∂τSσr=∫d0−σττ2−r(v,Zi,Ξi) dv+∫0aσττ2−r(v,Zr,Ξr) dv,∂τSorientedi≤−∣a−d∣,∂τSσr≤−(a+d).(B78) \begin{gathered} \partial_\tau S^i_\sigma =\int_d^a\frac{\sigma\tau}{\sqrt{\tau^2-r(v,Z,\Xi)}}\,dv,\\ \partial_\tau S^r_\sigma =\int_d^0\frac{-\sigma\tau}{\sqrt{\tau^2-r(v,Z_i,\Xi_i)}}\,dv\\ \qquad+\int_0^a\frac{\sigma\tau}{\sqrt{\tau^2-r(v,Z_r,\Xi_r)}}\,dv,\\ \partial_\tau S^i_{\mathrm{oriented}}\leq-|a-d|,\\ \partial_\tau S^r_\sigma\leq-(a+d). \end{gathered} \tag{B78} The last line uses r≥0r\geq0 along the retained real metric flows, so ∣τ∣/τ2−r≥1|\tau|/\sqrt{\tau^2-r}\geq1. On the lower incident leg reverse both the integration direction and the root sign. The initial plane phase is independent of τ\tau. These arguments also prove all smooth parameter derivatives on each incident side and on the reflected family.

Let θ∈Cc∞({τ:τ2∈J∘})\theta\in C_c^\infty(\{\tau:\tau^2\in J^\circ\}). At this point θ\theta need not be even. The cutoff Qh(d,τ2)Q_h(d,\tau^2) is the one used above. Define the tangential-operator-valued source and normal kernel by Qh(t;d)=(2πh)−1∫eitτ/h⋅θ(τ)Qh(d,τ2) dτ,KhD(t;a,d)=h22πh∫eitτ/hθ(τ)⋅G^σD(a,d;τ2)Qh(d,τ2) dτ,σ=−sgn⁡τ.(B79) \begin{gathered} \mathcal Q_h(t;d) =(2\pi h)^{-1}\int e^{it\tau/h}\\ \qquad\cdot\theta(\tau)Q_h(d,\tau^2)\,d\tau,\\ K_h^D(t;a,d) =\frac{h^2}{2\pi h}\int e^{it\tau/h}\theta(\tau)\\ \qquad\cdot\widehat G^D_\sigma(a,d;\tau^2) Q_h(d,\tau^2)\,d\tau,\\ \sigma=-\operatorname{sgn}\tau. \end{gathered} \tag{B79} These compact-frequency integrals define ordinary smooth time families of the normal operator kernels, with the previously specified source-slice distributional meaning. Put Ph=(hDa)2+Th(a)\mathscr P_h=(hD_a)^2+T_h(a). Since the extension in (B69) is independent of energy except for −E-E, (B76) gives (∂t2+h−2Ph)KhD=δ(a−d)Qh(t;d),KhD(t;0,d)=0.(B80) \begin{gathered} (\partial_t^2+h^{-2}\mathscr P_h)K_h^D =\delta(a-d)\mathcal Q_h(t;d),\\ K_h^D(t;0,d)=0. \end{gathered} \tag{B80} Indeed applying ∂t2+h−2Ph\partial_t^2+h^{-2}\mathscr P_h under the integral yields h−2Lh(τ2)h^{-2}L_h(\tau^2); its h−2h^{-2} cancels precisely the h2h^2 in (B79). This proves the physical-time source prefactor. It is an equation for the chosen extended normal expression, not yet the actual global Dirichlet operator.

For every fixed ε>0\varepsilon>0, bounded time interval with t≤−εt\leq-\varepsilon, and every prescribed finite derivative collection, the reflected kernel and each ordinary incident side satisfy ∣∂αKhr∣+∣∂αKhi∣≤CN,α,εhN.(B81) |\partial^\alpha K_h^r|+ |\partial^\alpha K_h^i|\leq C_{N,\alpha,\varepsilon}h^N. \tag{B81} To prove it, replace the exact operators by their phase kernels to a sufficiently high finite accuracy using (B63), (B74) and (B77). Their inverse factors carry the explicit h−1h^{-1}, while (B79) carries the other fixed powers; increasing the accuracy absorbs all of them and all chosen derivatives. For a phase term, (B78) gives ∣∂τ(tτ+S)∣≥ε|\partial_\tau(t\tau+S)|\geq\varepsilon. Integrate repeatedly in τ\tau with (h/i)(t+∂τS)−1∂τ(h/i)(t+\partial_\tau S)^{-1}\partial_\tau. All amplitudes have smooth compact temporal support, so there are no endpoint terms. The coefficient and its derivatives are uniformly bounded on the compact parameters. Each integration supplies hh; each preassigned ordinary derivative loses only a fixed power. This proves (B81), uniformly as either normal distance tends to zero. Across a=da=d, derivatives are distributions; their jump coefficients have the same rapid bounds by the same compact temporal integration. The reflected kernel itself is smooth through that slice. This is rapid decay before negative times separated from zero, not exact causal support for a temporally band-limited function.

19. The actual retarded spectral family with a smooth temporal cutoff

We now give the corresponding exact identity for the actual compact Dirichlet operator PP. This fixes what the normal construction must match. Let Pej=λjejPe_j=\lambda_je_j, κj=λj>0\kappa_j=\sqrt{\lambda_j}>0, and Πjf=(f,ej)ej\Pi_j f=(f,e_j)e_j, with the eigenbasis and exact domains proved in Compact positive inverses and diagonal domains, equations (1)–(2), and applied to this realization in Dirichlet wave regularization, equations (W1)–(W8). Let Qh(E)Q_h(E) be any smooth operator family on L2(X)L^2(X), supported in the fixed energy interval after multiplication by the cutoff below, with uniform operator bounds for every required energy derivative. The local tangential cutoffs used here have those bounds after fixed coordinate and density cutoffs: apply (N17) on each normal slice and integrate its squared estimate in the normal variable. Smooth density multipliers on the compact chart only change its constant.

Assume now that θ\theta is even, and write Θ(E)=θ(E)\Theta(E)=\theta(\sqrt E). In this section Qh(t)\mathcal Q_h(t) is the full spatial operator defined by the first integral in (B79), with this Qh(E)Q_h(E). Define S(u)=sin⁡(uP)P,KhP(t)=∫0∞S(u)Qh(t−u) du.(B82) \begin{gathered} S(u)=\frac{\sin(u\sqrt P)}{\sqrt P},\\ K_h^P(t)=\int_0^\infty S(u)\mathcal Q_h(t-u)\,du. \end{gathered} \tag{B82} These are actual operators, not resolvents evaluated at an eigenvalue. By the eigenbasis, ∥S(u)∥≤λmin⁡−1/2\|S(u)\|\leq\lambda_{\min}^{-1/2} and ∥S′(u)∥≤1\|S'(u)\|\leq1. Integration by parts in the compact τ\tau integral gives, for all fixed k,Ak,A, ∥∂tkQh(t)∥≤Ck,Ah−1−k(1+∣t∣/h)−A\|\partial_t^k\mathcal Q_h(t)\|\leq C_{k,A}h^{-1-k}(1+|t|/h)^{-A}. For ∣t∣≤h|t|\leq h use the absolute integral; for ∣t∣>h|t|>h integrate AA times and use the bounded energy derivatives. Thus (B82) and every fixed time derivative converge in operator norm. Moving one derivative from Qh\mathcal Q_h onto SS, with S(0)=0S(0)=0, gives KhP′(t)=∫0∞cos⁡(uP)Qh(t−u) duK_h^{P\prime}(t)=\int_0^\infty\cos(u\sqrt P)\mathcal Q_h(t-u)\,du. Interpret this last integral strongly on each input vector; its tails converge in operator norm by the integrable bound. No operator-norm continuity of the cosine group is assumed. The original integral and its derivatives defined with S(u)∂tkQhS(u)\partial_t^k\mathcal Q_h converge in operator norm because SS is norm continuous, by ∥S(u)−S(v)∥≤∣u−v∣\|S(u)-S(v)\|\leq|u-v|.

For a finite eigenfunction projection, two scalar integrations by parts give (∂t2+λj)ΠjKhP=ΠjQh(\partial_t^2+\lambda_j)\Pi_j K_h^P=\Pi_j\mathcal Q_h. Both KhP′′K_h^{P\prime\prime} and Qh\mathcal Q_h are bounded L2L^2-valued operators by the preceding estimates. The exact weighted-sum characterization of D(P)D(P) therefore shows, for every input, KhP(t)f∈D(P)K_h^P(t)f\in D(P) and (∂t2+P)KhP=Qh,KhP(t)f∣∂X=0,∥∂tkKhP(t)∥2→2=O(hN)(t≤−ε).(B83) \begin{gathered} (\partial_t^2+P)K_h^P=\mathcal Q_h,\\ K_h^P(t)f|_{\partial X}=0,\\ \|\partial_t^kK_h^P(t)\|_{2\to2}=O(h^N) \quad(t\leq-\varepsilon). \end{gathered} \tag{B83} For the last bound, u≥0u\geq0 implies ∣t−u∣≥ε+u|t-u|\geq\varepsilon+u. Integrating the preceding rapid bound for Qh\mathcal Q_h against the bounded sine operator proves any power by choosing AA large. The estimate is uniform on fixed negative time sets. The boundary condition follows from the proved domain of the original Dirichlet realization. The operator PP was not replaced by the normal extension.

20. The factor of two and the spectral band

Evenness in τ\tau makes Qh\mathcal Q_h even in time. Oddness of SS then gives the exact identity KhP(t)−KhP(−t)=∫RS(u)Qh(t−u) du=∑jΘ(h2λj)sin⁡(tκj)κjΠjQh(h2λj).(B84) \begin{gathered} K_h^P(t)-K_h^P(-t) =\int_{\mathbb R}S(u)\mathcal Q_h(t-u)\,du\\ =\sum_j\Theta(h^2\lambda_j) \frac{\sin(t\kappa_j)}{\kappa_j} \Pi_jQ_h(h^2\lambda_j). \end{gathered} \tag{B84} The first equality follows by changing uu to −u-u in the negative half of the absolutely convergent integral. For the second, project onto eje_j and write the sine as its two exponentials. Fourier inversion for the smooth compact operator-valued function θ(τ)Qh(τ2)\theta(\tau)Q_h(\tau^2), tested against any two L2L^2 vectors, evaluates it at τ=±hκj\tau=\pm h\kappa_j. Evenness makes both values equal. The ordinary Fourier inversion proof already used in the programme applies to these scalar smooth compact functions. Their derivative bounds justify the integrals. Only finitely many eigenvalues lie in the fixed scaled band for each h>0h>0, so the resulting sum is finite. Equality of every eigencomponent proves the operator identity. No commutation of Qh(E)Q_h(E) with PP has been made: the projection is on the left in the displayed order.

Differentiating the finite sum gives KhP′(t)+KhP′(−t)=∑jΘ(h2λj)cos⁡(tκj)ΠjQh(h2λj),2KhP′(0)=∑jΘ(h2λj)ΠjQh(h2λj).(B85) \begin{gathered} K_h^{P\prime}(t)+K_h^{P\prime}(-t)\\ =\sum_j\Theta(h^2\lambda_j)\cos(t\kappa_j) \Pi_jQ_h(h^2\lambda_j),\\ 2K_h^{P\prime}(0) =\sum_j\Theta(h^2\lambda_j)\Pi_jQ_h(h^2\lambda_j). \end{gathered} \tag{B85} In particular a smooth temporal cutoff of the retarded sine family contributes one half of this band operator at the zero-time derivative. Omitting that factor would give the wrong spectral coefficient. With Qh=IQ_h=I, the right side is precisely the smooth spectral band multiplier; with a varying Qh(E)Q_h(E), (B85) specifies the exact ordered band operator that must be matched locally.

The normal reflected family has the same prefactor. Define N^h,Θr\widehat{\mathcal N}_{h,\Theta}^r by the right side below, with H^\widehat H from (B77). Differentiating the reflected part of (B79), using σ=−sgn⁡τ\sigma=-\operatorname{sgn}\tau, and then changing E=τ2E=\tau^2 on each half-axis gives 2γ(d,y)∂tKhr(0;d,y;d,y)=N^h,Θr(d,y),N^h,Θr(d,y)=12πh γ(d,y)⋅∑σ∫JΘ(E)H^σ,h(d,d;E)(y,y) dE.(B86) \begin{gathered} \frac{2}{\gamma(d,y)}\partial_tK_h^r(0;d,y;d,y) =\widehat{\mathcal N}_{h,\Theta}^r(d,y),\\ \widehat{\mathcal N}_{h,\Theta}^r(d,y) =\frac{1}{2\pi h\,\gamma(d,y)}\\ \qquad\cdot\sum_\sigma\int_J\Theta(E) \widehat H_{\sigma,h}(d,d;E)(y,y)\,dE. \end{gathered} \tag{B86} For the sign and constant, (B77) says G^σrQh=−σ(ih)−1H^σ,h\widehat G_\sigma^rQ_h=-\sigma(ih)^{-1}\widehat H_{\sigma,h}. The time derivative in (B79) therefore has coefficient −στ/(2πh)=∣τ∣/(2πh)-\sigma\tau/(2\pi h)=|\tau|/(2\pi h). On each half-axis ∣τ∣ ∣dτ∣=dE/2|\tau|\,|d\tau|=dE/2. The additional factor two on the left of (B86) gives exactly the displayed 1/(2πh)1/(2\pi h). The diagonal gauge factors cancel as in Section 15, and division by γ\gamma is the same metric-volume conversion. Thus the normal source jump and the actual retarded spectral identity give consistent coefficients.

The smooth temporal cutoff in Sections 18–20 is essential to their rapid negative-time bounds. A sharp upper energy endpoint cannot be substituted into their integration-by-parts proof: it would add endpoint terms. Equation (B86) fixes the local energy-density normalization for smooth tests. The sharp cumulative endpoint in (B67)–(B68) retains its separate energy-endpoint analysis from Lemma 5.1. Neither calculation alone identifies the normal extension with the actual spectral projector.

21. Comparing the normal and physical waves

Equations (B76)–(B86) fix the normal Green equation, its phase representation, temporal orientation and source normalization. To identify this family with the physical wave, replace Ph\mathscr P_h in (B80) by the actual gauged h2Ph^2P and estimate the extension and position-cutoff errors. Sections 22–27 perform this comparison in energy norms and then control the diagonal uniformly at the wall. Sections 28–30 treat the complementary frozen model. The full-frequency argument in Sections 31–38 proves (B16), including the regions not covered by the near-normal cutoff.

22. Source columns with uniform energy norms at the wall

We now compare the normal construction with the actual wave for a retained near-normal right cutoff. The estimates will hold for every fixed target and time derivative, uniformly in the source point (d,y)(d,y), including its limit at the wall. No estimate for arbitrary normal derivatives of a point source is assumed. Reduce the retained collar and patches once so that all larger cutoffs fit inside the phase-construction region of Sections 6–20; write d0d_0 for this smaller retained collar width.

First identify the energy space of the original positive Dirichlet operator. Use its Hermitian form qq and the Gårding bound (10)–(11) in Smooth Dirichlet regularity, together with the actual eigenbasis Pej=λjejPe_j=\lambda_je_j. For a large fixed CC, the inner product q+C(⋅,⋅)q+C(\cdot,\cdot) is equivalent to H01H_0^1. Finite eigenfunction sums are dense in this inner product: a vector orthogonal to every eje_j has (λj+C)(u,ej)=0(\lambda_j+C)(u,e_j)=0, by the weak form identity, and is zero by completeness of the L2L^2 basis. The Hilbert projection argument then makes their closed span the whole energy space. On those sums q(u,u)=∑jλj∣uj∣2q(u,u)=\sum_j\lambda_j|u_j|^2. Passage in the form norm and strict positivity λj≥λmin⁡>0\lambda_j\geq\lambda_{\min}>0 show that this is an equivalent complete norm on H01H_0^1. Write ED1\mathcal E_D^1 for this normed energy space and ED−1\mathcal E_D^{-1} for its anti-dual. This notation leaves the shifted HDs\mathcal H_D^s norms of (W3) unchanged. With the anti-dual convention of (W4), the exact coefficient norms are ∥u∥ED12=∑jλj∣uj∣2≍∥u∥H12,u∈H01,∥f∥ED−12=∑jλj−1∣fj∣2,∥P−1f∥ED1=∥f∥ED−1.(B87) \begin{gathered} \|u\|_{\mathcal E_D^1}^2=\sum_j\lambda_j|u_j|^2 \asymp\|u\|_{H^1}^2,\quad u\in H_0^1,\\ \|f\|_{\mathcal E_D^{-1}}^2=\sum_j\lambda_j^{-1}|f_j|^2,\\ \|P^{-1}f\|_{\mathcal E_D^1} =\|f\|_{\mathcal E_D^{-1}}. \end{gathered} \tag{B87} For the dual formula, first test on finite eigenfunction sums and use weighted Cauchy–Schwarz. Conversely the finite choices uj=λj−1fju_j=\lambda_j^{-1}f_j, with the anti-dual convention, recover every finite partial sum of the norm; density just proved extends the functional to all of H01H_0^1. This proves the identification, rather than presuming a fractional-domain theorem. The cosine multipliers have norm at most one on this dual space.

Write qh(d,z,y,E)q_h(d,z,y,E) for the kernel of Qh(d,E)Q_h(d,E) in Section 14; its symbol is fixed smooth compact tangential phase data, with uniformly bounded parameter derivatives. In a fixed coordinate strip, the elementary slice trace bound and the kernel estimate give ∥v(d,⋅)∥Lz2≤C∥v∥H1,0≤d≤d0,∥∂Ejqh(d,⋅,y,E)∥Lz2≤Cjh−m/2,m=n−1,∥fh,E,d,y∥ED−1≤Ch−m/2.(B88) \begin{gathered} \|v(d,\cdot)\|_{L^2_z}\leq C\|v\|_{H^1}, \quad 0\leq d\leq d_0,\\ \|\partial_E^j q_h(d,\cdot,y,E)\|_{L^2_z} \leq C_jh^{-m/2},\\ m=n-1,\\ \|f_{h,E,d,y}\|_{\mathcal E_D^{-1}} \leq C h^{-m/2}. \end{gathered} \tag{B88} Here, in coordinate half-density coefficients, the source in the last line is fh,E,d,y(a,z)=δ(a−d)κ(d,y)κ(d,z)−1qh(d,z,y,E)f_{h,E,d,y}(a,z)=\delta(a-d)\kappa(d,y)\kappa(d,z)^{-1}q_h(d,z,y,E), extended by zero past the artificial chart edges. The smooth nonvanishing normal gauge κ\kappa and its inverse have bounded derivatives on the larger chart. A fixed input cutoff, equal to one on all retained (d,y)(d,y), defines the corresponding global source operator; it is suppressed in this formula. The last estimate also holds after every fixed energy derivative.

For the first line of (B88), apply the fundamental theorem to v(d,z)−v(s,z)v(d,z)-v(s,z), use Cauchy–Schwarz on the fixed strip, and average ss over that strip. The resulting constant is independent of dd. Smooth approximation up to the wall, proved in Section 1 of the smooth Dirichlet reading, extends it to H1H^1. For the second line, integration by parts in the compact symbol frequency gives ∣∂Ejqh∣≤Cj,Ah−m(1+∣z−y∣/h)−A|\partial_E^j q_h|\leq C_{j,A}h^{-m}(1+|z-y|/h)^{-A}. Squaring and substituting z−y=hwz-y=hw proves the bound. Pairing this Lz2L^2_z kernel with the slice trace, and then using (B87), proves the final assertion. Smooth gauge factors change only constants. Thus the estimate is uniform as an interior source approaches the wall. At the wall its functional on H01H_0^1 is zero; we do not insert an interior delta source at a boundary point.

23. Retarded columns in the energy space

Use a fixed even θ\theta as in Section 19 and set Θ(E)=θ(E)\Theta(E)=\theta(\sqrt E). For each retained source define fh(t)=(2πh)−1∫eitτ/h⋅θ(τ)fh,τ2,d,y dτ,∥∂tkfh(t)∥ED−1≤Ck,Ah−m/2−1−k(1+∣t∣/h)−A.(B89) \begin{gathered} f_h(t)=(2\pi h)^{-1}\int e^{it\tau/h}\\ \qquad\cdot\theta(\tau)f_{h,\tau^2,d,y}\,d\tau,\\ \|\partial_t^k f_h(t)\|_{\mathcal E_D^{-1}}\\ \leq C_{k,A}h^{-m/2-1-k}(1+|t|/h)^{-A}. \end{gathered} \tag{B89} Absolute integration for ∣t∣≤h|t|\leq h and repeated integration by parts for ∣t∣>h|t|>h, using (B88), prove the estimate. All constants are uniform in the source. These are strong Hilbert-space integrals of smooth compact-parameter families.

The actual retarded column is the sine convolution of (B82), now in this energy dual. It has the more regular representation uhP(t)=∫0∞S(v)fh(t−v) dv,uhP(t)=P−1fh(t)−P−1∫0∞cos⁡(vP)fh′(t−v) dv,uhP∈C∞(R;H01),∥∂tkuhP(t)∥H1=O(hN),t≤−ε.(B90) \begin{gathered} u_h^P(t)=\int_0^\infty S(v)f_h(t-v)\,dv,\\ u_h^P(t)=P^{-1}f_h(t)\\ -P^{-1}\int_0^\infty\cos(v\sqrt P)f_h'(t-v)\,dv,\\ u_h^P\in C^\infty(\mathbb R;H_0^1),\\ \|\partial_t^k u_h^P(t)\|_{H^1}=O(h^N), \quad t\leq-\varepsilon. \end{gathered} \tag{B90} The first integral converges in L2L^2, since S(v):ED−1→L2S(v):\mathcal E_D^{-1}\to L^2 is bounded by one in the coefficient norms. The second follows by one scalar integration by parts on each eigencomponent, using S(v)=−P−1∂vcos⁡(vP)S(v)=-P^{-1}\partial_v\cos(v\sqrt P); its boundary term is P−1fh(t)P^{-1}f_h(t). The cosine is strongly continuous and bounded on the energy dual, so the second integral converges there by (B89). Equation (B87) makes the displayed equality an H01H_0^1 identity. The same argument for every time derivative proves the stated regularity and a fixed polynomial bound in h−1h^{-1} on bounded time intervals. For t≤−εt\leq-\varepsilon, use ∣t−v∣≥ε+v|t-v|\geq\varepsilon+v in (B89) and choose AA arbitrarily large. This proves its last line for every prescribed N,kN,k.

Eigencomponent testing gives (∂t2+P)uhP=fh(\partial_t^2+P)u_h^P=f_h in the energy dual and the actual homogeneous Dirichlet condition. The even-source identities (B84)–(B85) remain valid columnwise: their scalar Fourier calculations apply to each eigencomponent, and only finitely many components survive the scaled band. In particular their right side is the actual kernel column of ∑jΘ(h2λj)cos⁡(tκj)ΠjQhκ(h2λj)\sum_j\Theta(h^2\lambda_j)\cos(t\kappa_j)\Pi_jQ_h^\kappa(h^2\lambda_j), where QhκQ_h^\kappa denotes the embedded family κ−1Qhκ\kappa^{-1}Q_h\kappa. This preserves the operator order.

24. The actual extension error and its odd part

Keep the particular extension (B69). On the larger chart the difference from the actual gauged operator is tangential: Δh(a)=h2κPκ−1−((hDa)2+Th(a)),Zσ,h(a,d;E)=Δh(a)G^σD(a,d;E)Qh(d,E),∂αZσ,h(a,d;E)(z,y)=O(hN).(B91) \begin{gathered} \Delta_h(a)=h^2\kappa P\kappa^{-1}\\ -\bigl((hD_a)^2+T_h(a)\bigr),\\ Z_{\sigma,h}(a,d;E)=\Delta_h(a) \widehat G^D_\sigma(a,d;E)Q_h(d,E),\\ \partial^\alpha Z_{\sigma,h}(a,d;E)(z,y)=O(h^N). \end{gathered} \tag{B91} The kernel estimate holds for any prescribed finite derivatives on either closed incident side separately and for the reflected part smoothly; LL in the finite root construction is chosen sufficiently large. The source point and all retained parameters have uniform constants. In particular its value is continuous across a=da=d. Higher normal derivatives across that slice are not asserted to be ordinary functions.

Here is the operator error proof. The left symbol of Δh\Delta_h is a degree-two polynomial tangential differential symbol minus a compact symbol. It and all its derivatives vanish on a neighborhood of the retained phase tubes. Apply the exact finite differential phase action to the polynomial part and (B53) to the compact part. Their coefficients cancel to every chosen finite order because they are evaluated at the actual phase gradient in that neighborhood. The differential action has no terms past its degree; the compact part has the bounded differentiated remainder of (B53). Thus their action on every incident-side or reflected phase kernel is arbitrarily small with all prescribed ordinary derivatives. The true kernel differs by arbitrarily accurate weighted smoothing remainders, by (B74)–(B77). Allow two extra semiclassical Sobolev derivatives before applying Δh\Delta_h, and use its degree-two differential bound and the bounded-symbol estimate. Equation (B57) converts the resulting weighted norm into the same ordinary kernel bounds. Increasing the accuracy absorbs the Green factor h−1h^{-1} and every fixed parameter loss. This proves (B91) for the actual operators, including their tangential frequency tails.

The energy independence of Δh\Delta_h is useful here. Since θ\theta is even, the odd time part of ΔhKhD\Delta_h K_h^D involves the orientation difference G^−D−G^+D\widehat G^D_- -\widehat G^D_+. By (B76) that difference is jointly smooth in both normal variables. It follows that Dh(t)=ΔhKhD(t),∂a,z,tα{Dh(t)−Dh(−t)}=O(hN).(B92) \begin{gathered} \mathcal D_h(t)=\Delta_hK_h^D(t),\\ \partial^\alpha_{a,z,t} \{\mathcal D_h(t)-\mathcal D_h(-t)\}\\ =O(h^N). \end{gathered} \tag{B92} for the kernel coefficients at (a,z;d,y)(a,z;d,y) on the entire retained normal rectangle, including a=da=d and its wall limit. To verify its size, integrate (B91) on each side with the compact temporal profile, retaining the fixed powers of hh. The derivatives of the two side formulas match, by the exact Cauchy uniqueness in (B76); their bounds therefore extend across the slice. This proves the asserted ordinary derivative bounds for the odd part without treating small delta coefficients as pointwise-small functions.

25. A forced local energy comparison

Choose a smooth position cutoff β(a,z)\beta(a,z) supported inside the larger chart, equal to one on a neighborhood of all source output supports in (B88) and on the retained target patch. All phase tubes through its support remain inside the root agreement region. Its derivatives are supported outside a fixed smaller neighborhood UU of the target patch. Restore the normal gauge and define uhN(t;a,z)=β(a,z)κ(a,z)−1⋅KhD(t;a,z;d,y)κ(d,y),Dh=uhP−uhN,(∂t2+P)Dh=Fhsmall+Fhedge,Fhsmall=−βκ−1h−2ΔhKhD κ(d,y),Fhedge=−[P,β]κ−1KhD κ(d,y).(B93) \begin{gathered} u_h^N(t;a,z)=\beta(a,z)\kappa(a,z)^{-1}\\ \qquad\cdot K_h^D(t;a,z;d,y)\kappa(d,y),\\ D_h=u_h^P-u_h^N,\\ (\partial_t^2+P)D_h=F_h^{\rm small}+F_h^{\rm edge},\\ F_h^{\rm small}=-\beta\kappa^{-1}h^{-2} \Delta_hK_h^D\,\kappa(d,y),\\ F_h^{\rm edge}=-[P,\beta]\kappa^{-1} K_h^D\,\kappa(d,y). \end{gathered} \tag{B93} The source cancels exactly: the normal equation has the source δ(a−d)Qh\delta(a-d)\mathcal Q_h, and β=1\beta=1 on its compact output support. Coordinate half-density identifications introduce precisely the displayed gauge factors; fixed smooth trivializations give equivalent norms. The formula has no source truncation remainder.

Both columns are C∞C^\infty in time with values in H01H_0^1, with polynomial bounds in h−1h^{-1}. For the normal column this follows from its continuous incident values, bounded piecewise first normal derivatives, tangential smoothing and exact zero wall value; its position support is compact. The zero-trace characterization in the smooth Dirichlet reading then gives H01H_0^1. For the actual column use (B90). Their negative-time data have arbitrarily small energy norms, by (B81) and (B90). From (B91) and the compact position support, ∥∂tkFhsmall(t)∥L2=O(hN),supp⁡Fhedge⊆supp⁡coeff[P,β],∥∂tkDh(−2T)∥H1+∥∂tk+1Dh(−2T)∥2=O(hN).(B94) \begin{gathered} \|\partial_t^k F_h^{\rm small}(t)\|_{L^2}=O(h^N),\\ \operatorname{supp}F_h^{\rm edge} \subseteq\operatorname{supp}_{\rm coeff}[P,\beta],\\ \|\partial_t^k D_h(-2T)\|_{H^1}\\ +\|\partial_t^{k+1}D_h(-2T)\|_2=O(h^N). \end{gathered} \tag{B94} Here supp⁡coeff[P,β]\operatorname{supp}_{\rm coeff}[P,\beta] is the union of the supports of its differentiated-cutoff coefficients; it is disjoint from UU. All bounds hold for every finite k,Nk,N, after increasing the construction accuracy. The edge term need only have a polynomial norm bound. Each forcing is C∞C^\infty in time with values in L2L^2. Equation (B93), Dh∈C∞H01D_h\in C^\infty H_0^1, and the actual Dirichlet H2H^2 estimate therefore give Dh∈C∞(H2∩H01)D_h\in C^\infty(H^2\cap H_0^1). This justifies the strong energy test below.

For completeness the local estimate permits this forcing and a general chart neighborhood. Choose a smooth real function b(x)b(x), positive on a compact smaller target patch KK, with its positive set contained in UU. Choose V≥sup⁡p(x,db)V\geq\sup\sqrt{p(x,db)}, and take T>0T>0 so small that 4VT<12inf⁡Kb4VT<\frac12\inf_K b. With the increasing smooth function χ\chi from (T159), put φ(t,x)=χ(b(x)−V(t+2T))\varphi(t,x)=\chi(b(x)-V(t+2T)), for −2T≤t≤2T-2T\leq t\leq2T. The energy identity (T158), now with the additional term Re⁡(φFDh,t‾)\operatorname{Re}(\varphi F\overline{D_{h,t}}), gives Eφ′(t)≤CEφ(t)+C∥φFhsmall(t)∥22,∥∂tkDh(t)∥H1(K)+∥∂tk+1Dh(t)∥L2(K)=O(hN),∣t∣≤T.(B95) \begin{gathered} E_\varphi'(t)\leq C E_\varphi(t)\\ +C\|\sqrt\varphi F_h^{\rm small}(t)\|_2^2,\\ \|\partial_t^k D_h(t)\|_{H^1(K)}\\ +\|\partial_t^{k+1}D_h(t)\|_{L^2(K)}=O(h^N),\\ |t|\leq T. \end{gathered} \tag{B95} Indeed φt=−Vχ′\varphi_t=-V\chi', dφ=χ′dbd\varphi=\chi'db, so the time-weight and flux terms have nonpositive sum by the same positive-form Cauchy–Schwarz argument as (T159). The lower coefficients contribute at most CEφCE_\varphi. Bound the forcing product by a constant times φ(∣F∣2+∣Dh,t∣2)\varphi(|F|^2+|D_{h,t}|^2). The edge forcing vanishes on this weight's support. Integrate the resulting inequality from −2T-2T, using (B94). The weight has a fixed positive lower bound on KK, giving the second line. Apply this same argument to each time derivative of (B93), since PP is time independent. No propagation-of-wavefront assertion is used as a quantitative bound.

26. From energy to the boundary diagonal

Put Wh(t)=Dh(t)−Dh(−t)W_h(t)=D_h(t)-D_h(-t). On UU, where β=1\beta=1, its equation and boundary value are (∂t2+P)Wh=Fhsmall(t)−Fhsmall(−t),Wh∣∂X=0,∥∂tkWh(t)∥Hs(K′)=O(hN)(∣t∣≤T)(B96) \begin{gathered} (\partial_t^2+P)W_h =F_h^{\rm small}(t)-F_h^{\rm small}(-t),\\ W_h|_{\partial X}=0,\\ \|\partial_t^kW_h(t)\|_{H^s(K')}=O(h^N) \quad(|t|\leq T) \end{gathered} \tag{B96} for every fixed k,s,Nk,s,N, on any fixed target patch K′K' compactly inside KK relative to the manifold with boundary. The source remains uniform in the full retained collar.

Here are the regularity and size arguments for the last line. The odd forcing has all target spatial and time derivatives O(hN)O(h^N), by (B92), including the smooth gauge and position factors on UU. Equation (B95) supplies the initial H1H^1 bounds for every fixed number of time derivatives. On finitely many nested interior or boundary half-patches, apply the local estimates of Sections 2–3 of Smooth Dirichlet regularity to P∂tkWh=∂tkFodd−∂tk+2WhP\partial_t^kW_h=\partial_t^k F_{\rm odd}-\partial_t^{k+2}W_h. Their first step gives H2H^2 from the L2L^2 right side and the controlled local H1H^1 norm. The higher steps give Hr+2H^{r+2} from an HrH^r right side and the lower local norms. Induct simultaneously on spatial order for the finitely many needed time derivatives; start with enough of those derivatives in (B95). Every cutoff commutator is one order lower and is controlled on the preceding larger patch. The number of patches and derivatives is finite for a prescribed s,ks,k, so the constants do not depend on h,d,yh,d,y. All traces remain zero and every membership assertion is obtained before applying the next estimate. This proves (B96).

Use the bounded half-space extensions in Lemma 1.3 of that reading and Fourier Cauchy–Schwarz with s>n/2+js>n/2+j. They bound the first jj pointwise target derivatives by the HsH^s norm, uniformly up to the wall. Since ∂tWh=Dh′(t)+Dh′(−t)\partial_tW_h=D_h'(t)+D_h'(-t), the actual cosine band and the normal one satisfy Ch,Θ,QP(t)=∑jΘ(h2λj)cos⁡(tκj)⋅ΠjQhκ(h2λj),Ch,Θ,QN(t)=∂tuhN(t)+∂tuhN(−t),∣∂x,tα(Ch,Θ,QP−Ch,Θ,QN)∣≤Cα,NhN,∣t∣≤T.(B97) \begin{gathered} C_{h,\Theta,Q}^P(t) =\sum_j\Theta(h^2\lambda_j)\cos(t\kappa_j)\\ \qquad\cdot\Pi_jQ_h^\kappa(h^2\lambda_j),\\ C_{h,\Theta,Q}^N(t)= \partial_tu_h^N(t)+\partial_tu_h^N(-t),\\ |\partial_{x,t}^{\alpha} (C_{h,\Theta,Q}^P-C_{h,\Theta,Q}^N)|\\ \leq C_{\alpha,N}h^N,\quad |t|\leq T. \end{gathered} \tag{B97} The kernels in the last line of (B97) are evaluated at (t,x;d,y)(t,x;d,y). This is the required actual near-normal short-time comparison for a fixed smooth energy band and right cutoff. It includes pointwise diagonal evaluation and the wall limit. It does not assert a comparable theorem for the complementary phase regions. Source normal derivatives, which were not used, are not inferred from the target estimates.

27. The normal contribution with a sharp upper endpoint

We now apply the comparison without replacing a smooth temporal cutoff by a discontinuous one. On the diagonal x=(d,y)x=(d,y) in K′K', set Hh(E;d,y)=2[Ah(d,E)Qh(d,E)](y,y)+∑σ[H^σ,h(d,d;E)](y,y),Ch,Θ,QN(t;x,x)=12πh γ(d,y)⋅∫JΘ(E)cos⁡(tE/h)Hh(E;d,y) dE,∣Hh(E;d,y)∣≤Ch−m.(B98) \begin{gathered} \mathcal H_h(E;d,y)=2[A_h(d,E)Q_h(d,E)](y,y)\\ +\sum_\sigma[\widehat H_{\sigma,h}(d,d;E)](y,y),\\ C_{h,\Theta,Q}^N(t;x,x) =\frac{1}{2\pi h\,\gamma(d,y)}\\ \quad\cdot\int_J\Theta(E)\cos(t\sqrt E/h) \mathcal H_h(E;d,y)\,dE,\\ |\mathcal H_h(E;d,y)|\leq C h^{-m}. \end{gathered} \tag{B98} For the formula, the normalization (−σih)G^σDQh(-\sigma ih)\widehat G_\sigma^DQ_h gives AhQhA_hQ_h for each incident branch at a=da=d, and H^σ,h\widehat H_{\sigma,h} for its reflection. Adding the derivatives at t,−tt,-t in (B79) gives the cosine and the factor 1/(2πh)1/(2\pi h), exactly as in (B86). The two gauge factors cancel on the diagonal; γ−1\gamma^{-1} changes the coordinate half-density coefficient to density relative to dVgdV_g. The bound follows from (B58) and the compact-frequency phase kernel (B65), transferred by (B77). Their arbitrary small exact-kernel errors can be absorbed. The constants are uniform in distance.

Choose the nonnegative Schwartz smoothing function ρ\rho from (B4), with ρ^\widehat\rho supported in the time interval where (B97) holds. Let Fρ(s)=∫−∞sρ(v) dvF_\rho(s)=\int_{-\infty}^s\rho(v)\,dv, and define the actual short-time band contribution Ah(x)=1π∫ρ^(t)sin⁡(t/h)t⋅Ch,Θ,QP(t;x,x) dt,ah(E)=Fρ((1−E)/h)+Fρ((1+E)/h)−1.(B99) \begin{gathered} \mathscr A_h(x)=\frac1\pi\int \widehat\rho(t)\frac{\sin(t/h)}{t}\\ \qquad\cdot C_{h,\Theta,Q}^P(t;x,x)\,dt,\\ a_h(E)=F_\rho((1-\sqrt E)/h)\\ +F_\rho((1+\sqrt E)/h)-1. \end{gathered} \tag{B99} The quotient has its continuous value at zero. Equation (B97) permits replacing PP by NN, with any prescribed power of hh error: the time test costs at most C/hC/h, which is absorbed by increasing the kernel accuracy. Formula (B14) then identifies the resulting energy factor as ah(E)a_h(E).

On the fixed compact positive interval JJ, ∫J∣ah(E)−1{E≤1}∣ dE≤Ch.(B100) \int_J|a_h(E)-1_{\{E\leq1\}}|\,dE\leq C h. \tag{B100} The second FρF_\rho term differs from one by arbitrarily high powers of hh, uniformly on JJ. For the first put u=Eu=\sqrt E, whose Jacobian 2u2u is bounded there, and then v=(1−u)/hv=(1-u)/h. Its integral is bounded by Ch∫R∣Fρ(v)−1{v≥0}∣ dvCh\int_{\mathbb R}|F_\rho(v)-1_{\{v\geq0\}}|\,dv. Fubini for the nonnegative ρ\rho identifies this last integral with ∫∣s∣ρ(s) ds<∞\int|s|\rho(s)\,ds<\infty. Values at a single endpoint do not change these Lebesgue integrals. Combining (B98)–(B100) gives the actual-kernel formula Ah(x)=12πh γ(d,y)⋅∫J∩(−∞,1]Θ(E)Hh(E;d,y) dE+O(h1−n).(B101) \begin{gathered} \mathscr A_h(x)=\frac{1}{2\pi h\,\gamma(d,y)}\\ \quad\cdot\int_{J\cap(-\infty,1]}\Theta(E)\mathcal H_h(E;d,y)\,dE\\ +O(h^{1-n}). \end{gathered} \tag{B101} The error is h−1⋅O(h−m)⋅O(h)=O(h−m)h^{-1}\cdot O(h^{-m})\cdot O(h)=O(h^{-m}). This retains the sharp upper endpoint while using only the fixed smooth θ\theta in the wave comparison.

For example choose Θ\Theta supported above E0E_0, zero near E0E_0, and equal to one near 11. The incident principal term and the reflected frozen term in (B101) are Ih(x)=(2πh)−nγ(d,y)⋅∫E01∫Θ(E)q(d,y,η,E)λd dη dE,Rh,0(x)=−(2πh)−nγ(0,y)⋅∑σ∫E01∫e2iσdλ0/h⋅Θ(E)q(0,y,η,E)2λ0 dη dE,λd=E−r(d,y,η),λ0=E−r(0,y,η).(B102) \begin{gathered} I_h(x)=\frac{(2\pi h)^{-n}}{\gamma(d,y)}\\ \quad\cdot\int_{E_0}^1\int \frac{\Theta(E)q(d,y,\eta,E)}{\lambda_d}\,d\eta\,dE,\\ R_{h,0}(x)=-\frac{(2\pi h)^{-n}}{\gamma(0,y)}\\ \quad\cdot\sum_\sigma\int_{E_0}^1\int e^{2i\sigma d\lambda_0/h}\\ \qquad\cdot\frac{\Theta(E)q(0,y,\eta,E)}{2\lambda_0}\,d\eta\,dE,\\ \lambda_d=\sqrt{E-r(d,y,\eta)},\\ \lambda_0=\sqrt{E-r(0,y,\eta)}. \end{gathered} \tag{B102} Equation (B58) gives the incident formula, with its hh amplitude correction bounded absolutely by O(h1−n)O(h^{1-n}). For the reflected part use (B68) for the exact second-order family, as justified in (B77), with the smooth lower energy cutoff Θ\Theta and the actual upper endpoint 11. Thus Ah(x)=Ih(x)+Rh,0(x)+O(h1−n),0≤d≤d0.(B103) \begin{gathered} \mathscr A_h(x)=I_h(x)+R_{h,0}(x)\\ +O(h^{1-n}),\quad 0\leq d\leq d_0. \end{gathered} \tag{B103} Thus (B103) gives the actual contribution of the specified smooth lower energy band and near-normal right cutoff, with all lower-order terms, density factors and the sharp upper endpoint retained. The full-frequency estimate is proved in Sections 31–38.

28. Tangential energy coordinates through glancing

The roots used in Sections 6–27 stay separated. For the complementary region, the normal roots may merge. We first prove the exact frozen scalar model and its uniform estimates there. This is a necessary model calculation, not yet a comparison with the variable-coefficient wave.

Keep a compact positive energy interval JJ, and use α\alpha for the distance at which the coefficients are frozen. The observation distance dd will remain a separate variable. Put rα(y,η)=ηTG(α,y)η,m=n−1,q=q(α,y,η,E),supp⁡ηq⊆{ϵ≤∣η∣≤R},η⋅∂ηrα=2rα≥c∣η∣2.(B104) \begin{gathered} r_\alpha(y,\eta)=\eta^TG(\alpha,y)\eta,\quad m=n-1,\\ q=q(\alpha,y,\eta,E),\\ \operatorname{supp}_\eta q\subseteq \{\epsilon\leq|\eta|\leq R\},\\ \eta\cdot\partial_\eta r_\alpha=2r_\alpha \geq c|\eta|^2 . \end{gathered} \tag{B104} Here 0<ϵ<R0<\epsilon<R are fixed, qq is smooth with uniform derivatives, and all ordinary parameters range over compact sets. An additional parameter hh is allowed with the same bounds; its derivatives are not required. The last identity proves a quantitative tangential energy direction on the entire support, including the normal glancing set E=rαE=r_\alpha. In particular at least one component of ∂ηrα\partial_\eta r_\alpha has a fixed positive absolute lower bound on each member of a finite cover.

We give the integration argument rather than assuming a coarea formula at a merging normal root. On each smaller member of that cover, choose the component ηj\eta_j with nonzero derivative. The change of coordinates (ηj,η^)↦(v=rα(y,η),η^)(\eta_j,\widehat\eta)\mapsto(v=r_\alpha(y,\eta),\widehat\eta) is a smooth diffeomorphism there, by the parameter inverse theorem in Coordinate inverses and integration. Choose a smooth partition with support compactly inside these charts. A chart contribution to q dηq\,d\eta becomes bj(α,y,v,η^,E) dv dη^b_j(\alpha,y,v,\widehat\eta,E)\,dv\,d\widehat\eta, where the Jacobian factor is 1/∣∂ηjrα∣1/|\partial_{\eta_j}r_\alpha|. Extend bjb_j by zero outside its chart. All derivatives are uniformly bounded and its support is compact. The ordinary change-of-variables proof in that reading applies without an orientation sign because this is a density.

Define Aq(s,E;α,y)=∑j∫bj(α,y,E−s2,η^,E) dη^,Aq(−s,E;α,y)=Aq(s,E;α,y),∣∂s,E,α,yβAq∣≤Cβ,supp⁡sAq⊆[−C,C].(B105) \begin{gathered} A_q(s,E;\alpha,y)\\ =\sum_j\int b_j(\alpha,y,E-s^2,\widehat\eta,E)\,d\widehat\eta,\\ A_q(-s,E;\alpha,y)=A_q(s,E;\alpha,y),\\ |\partial_{s,E,\alpha,y}^{\beta}A_q|\leq C_\beta,\\ \operatorname{supp}_s A_q\subseteq[-C,C]. \end{gathered} \tag{B105} The bounds follow by differentiation under an integral on one fixed compact set. They hold through s=0s=0. In dimension n=2n=2, the η^\widehat\eta integral is an integral over zero variables, so it is simply evaluation and the same proof applies.

For fixed ss, this is precisely the density obtained by integrating qq on the tangential energy level rα=E−s2r_\alpha=E-s^2. More explicitly, if φ\varphi is a compactly supported smooth test in EE, change variables E=s2+vE=s^2+v in each chart to obtain ∫φ(E)Aq(s,E;α,y) dE=∫φ(s2+rα)⋅q(α,y,η,s2+rα) dη. \begin{gathered} \int\varphi(E)A_q(s,E;\alpha,y)\,dE\\ =\int\varphi(s^2+r_\alpha)\\ \qquad\cdot q(\alpha,y,\eta,s^2+r_\alpha)\,d\eta . \end{gathered} This identity defines any delta notation for the energy level used below. It proves smoothness by the tangential variable, with no division by the vanishing normal root.

29. The exact frozen Dirichlet resolvent and density

For fixed η,α,y\eta,\alpha,y, consider Hη=−h2∂a2+rα(y,η)H_\eta=-h^2\partial_a^2+r_\alpha(y,\eta) on the half-line a>0a>0, with the Dirichlet domain. Its realization is the odd restriction of the whole-line Fourier multiplier, as proved for the half-space in Section 1 of Reflection and the Dirichlet boundary coefficient. The same odd unitary map and the substitution of hDahD_a give that proof for every constant rαr_\alpha.

For Im⁡z>0\operatorname{Im}z>0, let κ=(z−rα)1/2\kappa=(z-r_\alpha)^{1/2} be the root with positive imaginary part. The inverse of Hη−zH_\eta-z has kernel Fκ(v)=eiκv/h,Gη(z;a,b)=i2hκ⋅(Fκ(∣a−b∣)−Fκ(a+b)),Gη(z;0,b)=0,[∂aGη]a=b=−h−2,∥(Hη−z)−1∥L2→L2≤(Im⁡z)−1.(B106) \begin{gathered} F_\kappa(v)=e^{i\kappa v/h},\\ G_\eta(z;a,b)=\frac{i}{2h\kappa}\\ \qquad\cdot\left(F_\kappa(|a-b|)-F_\kappa(a+b)\right),\\ G_\eta(z;0,b)=0,\\ [\partial_aG_\eta]_{a=b}=-h^{-2},\\ \|(H_\eta-z)^{-1}\|_{L^2\to L^2} \leq(\operatorname{Im}z)^{-1}. \end{gathered} \tag{B106} Indeed both exponentials solve the homogeneous ordinary differential equation off a=ba=b; their values are continuous and the displayed derivative jump gives a unit delta after multiplication by −h2-h^2. The image term enforces the zero boundary value. For compactly supported input the formula and its derivative decay at infinity and give the inverse equation. The odd Fourier multiplier has inverse symbol (s2+rα−z)−1(s^2+r_\alpha-z)^{-1}, bounded by (Im⁡z)−1(\operatorname{Im}z)^{-1}, which proves existence and that norm bound. Uniqueness follows either from this multiplier or by taking the imaginary part of the Dirichlet energy identity. Thus the kernel formula is the actual inverse of the frozen operator.

At glancing the quotient in this formula has a finite limit for fixed a,ba,b. Its first exponential difference is iκ(∣a−b∣−a−b)/h+O(κ2)i\kappa(|a-b|-a-b)/h+O(\kappa^2). Consequently lim⁡z→rαIm⁡z>0Gη(z;a,b)=h−2min⁡(a,b),1πIm⁡Gη(E+i0;d,d)=1−cos⁡(2dE−rα/h)2πhE−rα,E>rα.(B107) \begin{gathered} \lim_{\substack{z\to r_\alpha\\ \operatorname{Im}z>0}} G_\eta(z;a,b)\\ \qquad=h^{-2}\min(a,b),\\ \frac1\pi\operatorname{Im}G_\eta(E+i0;d,d)\\ =\frac{1-\cos(2d\sqrt{E-r_\alpha}/h)} {2\pi h\sqrt{E-r_\alpha}}, \quad E>r_\alpha. \end{gathered} \tag{B107} For E<rαE<r_\alpha the boundary value is real, so its imaginary part is zero. At E=rαE=r_\alpha the second expression extends by zero, since its numerator is O(E−rα)O(E-r_\alpha). This limit does not assert bounded derivatives of the separate normal roots.

For clarity the spectral-density interpretation does not rely on an unproved boundary-value theorem. The odd Fourier representation gives the diagonal normal spectral projector (2πh)−1∫s2+rα≤E(1−cos⁡(2ds/h)) ds(2\pi h)^{-1}\int_{s^2+r_\alpha\leq E}(1-\cos(2ds/h))\,ds. For E>rαE>r_\alpha, differentiation of its two endpoints gives exactly (B107). Below the threshold it is zero. The continuous cumulative function has no jump at the threshold and hence no atom there. This proves the asserted density directly from the unitary multiplier representation.

Restore the tangential Fourier factor (2πh)−m(2\pi h)^{-m} and the constant frozen volume density γ(α,y)\gamma(\alpha,y). Multiplying the spectral density at energy EE by q(α,y,η,E)q(\alpha,y,\eta,E), and then integrating in η\eta, yields Dh,q0(d,E;α,y)=(2πh)−nγ(α,y)⋅∫R(1−cos⁡(2ds/h))⋅Aq(s,E;α,y) ds.(B108) \begin{gathered} D^0_{h,q}(d,E;\alpha,y)\\ =\frac{(2\pi h)^{-n}}{\gamma(\alpha,y)}\\ \qquad\cdot\int_{\mathbb R} (1-\cos(2ds/h))\\ \qquad\cdot A_q(s,E;\alpha,y)\,ds . \end{gathered} \tag{B108} One can verify the equality by testing in EE and using the identity after (B105), followed by the odd Fourier formula. Every integral then has compact frequency support. The energy dependence of qq weights the spectral measure; it is not differentiated as if this were the derivative of a cumulative expression already containing q(E)q(E). This also fixes the factor of two from the two normal signs. The result is smooth in EE, with uniform tangential and coefficient-parameter derivatives, despite the possible glancing in its individual η\eta contributions.

30. A sharp energy endpoint and rapid decay of the complementary image

Let Θ\Theta be a fixed smooth lower energy cutoff on JJ, zero near a fixed E0>0E_0>0. For an upper endpoint ee in a fixed smaller positive interval in JJ, define Zq(s,e;α,y)=∫E0eΘ(E)Aq(s,E;α,y) dE,Ih,q0(α,y,e)=(2πh)−nγ(α,y)⋅∫Zq(s,e;α,y) ds,Rh,q0(d;α,y,e)=−(2πh)−nγ(α,y)⋅∫cos⁡(2ds/h)Zq(s,e;α,y) ds.(B109) \begin{gathered} Z_q(s,e;\alpha,y)\\ =\int_{E_0}^{e}\Theta(E)A_q(s,E;\alpha,y)\,dE,\\ \mathcal I^0_{h,q}(\alpha,y,e) =\frac{(2\pi h)^{-n}}{\gamma(\alpha,y)}\\ \qquad\cdot\int Z_q(s,e;\alpha,y)\,ds,\\ \mathcal R^0_{h,q}(d;\alpha,y,e) =-\frac{(2\pi h)^{-n}}{\gamma(\alpha,y)}\\ \qquad\cdot\int\cos(2ds/h)Z_q(s,e;\alpha,y)\,ds . \end{gathered} \tag{B109} The exact frozen weighted cumulative contribution is Ih,q0+Rh,q0\mathcal I^0_{h,q}+\mathcal R^0_{h,q}. Equation (B105) proves that ZqZ_q is smooth and compactly supported in ss, with every derivative in s,e,α,ys,e,\alpha,y uniformly bounded. Differentiation in ee evaluates a smooth integrand at that endpoint. Thus the sharp upper endpoint does not destroy smoothness in ss; that conclusion uses the tangential energy coordinate and the exclusion of η=0\eta=0.

For D=d/hD=d/h, repeated integration by parts in ss now gives Fq(D;α,y,e)=hnRh,q0(hD;α,y,e),∣∂D,e,α,yβFq∣≤Cβ,N(1+D)−N,D≥0,∣Rh,q0(d;d,y,e)−Rh,q0(d;0,y,e)∣≤Ch1−n,0≤d≤d0.(B110) \begin{gathered} \mathcal F_q(D;\alpha,y,e) =h^n\mathcal R^0_{h,q}(hD;\alpha,y,e),\\ |\partial_{D,e,\alpha,y}^{\beta}\mathcal F_q| \leq C_{\beta,N}(1+D)^{-N},\\ D\geq0,\\ \left|\begin{gathered} \mathcal R^0_{h,q}(d;d,y,e)\\ -\mathcal R^0_{h,q}(d;0,y,e) \end{gathered}\right| \leq C h^{1-n},\\ 0\leq d\leq d_0 . \end{gathered} \tag{B110} For the first line, DD derivatives multiply the compact amplitude by powers of ss. If D≥1D\geq1, write the cosine as two exponentials and integrate NN times; the boundary terms vanish because the amplitude is smooth and compactly supported. For D≤1D\leq1, use its bounded L1L^1 norm. Parameter derivatives of γ−1\gamma^{-1} are bounded and cause no change in this argument.

For the second line keep D=d/hD=d/h fixed while integrating the coefficient derivative in α\alpha from zero to dd. The first line bounds the difference by CNdh−n(1+d/h)−NC_N d h^{-n}(1+d/h)^{-N}. For N≥1N\geq1, this is at most Ch1−nC h^{1-n}. This estimate includes the glancing frequencies in (B104). It freezes all smooth coefficient and cutoff factors while retaining the observation distance in the oscillation.

Here is the exact model partition that connects this calculation to the earlier normal one. Choose a tangential cutoff q0q_0 equal to one on a sufficiently small neighborhood of η=0\eta=0, supported where the roots stay separated for E≥E0E\geq E_0. Choose a compact tangential cutoff χ\chi equal to one wherever rα≤sup⁡Jr_\alpha\leq\sup J, on all retained coefficient parameters, and equal to one on the support of q0q_0. Set q1=χ−q0q_1=\chi-q_0. Then q1q_1 has the support required in (B104), and q0+q1=1q_0+q_1=1 on every frozen energy shell in JJ.

For q0q_0, define Dh,q00D^0_{h,q_0} by the exact odd Fourier spectral density preceding (B108), with q0q_0 inserted. Its separated roots give the ordinary formula (2πh)−nγ−1∫q0(1−cos⁡(2dE−rα/h))/E−rα dη(2\pi h)^{-n}\gamma^{-1}\int q_0(1-\cos(2d\sqrt{E-r_\alpha}/h))/\sqrt{E-r_\alpha}\,d\eta. Thus this use of Dh,q00D^0_{h,q_0} does not assume that the tangential energy coordinates in (B105) exist at η=0\eta=0. Linearity of the exact odd Fourier formula gives ∑j=01∫E01Θ(E)Dh,qj0(d,E;α,y) dE=(2πh)−nγ(α,y)⋅∫{s2+rα≤1}Θ(s2+rα)⋅(1−cos⁡(2ds/h)) ds dη.(B111) \begin{gathered} \sum_{j=0}^1\int_{E_0}^{1} \Theta(E)D^0_{h,q_j}(d,E;\alpha,y)\,dE\\ \quad=\frac{(2\pi h)^{-n}}{\gamma(\alpha,y)}\\ \qquad\cdot\int_{\{s^2+r_\alpha\leq1\}} \Theta(s^2+r_\alpha)\\ \qquad\cdot(1-\cos(2ds/h))\,ds\,d\eta . \end{gathered} \tag{B111} Here Θ\Theta is extended by zero below E0E_0. The same partition may be made smoothly in the coefficient parameters by fixed slightly larger frequency cutoffs. No high-frequency remainder appears in this frozen identity because the spectral support itself bounds rαr_\alpha.

Equations (B104)–(B111) describe the complementary frozen contribution through glancing, its coefficient-freezing error and the complete frozen band partition. They do not compare the variable-coefficient complementary family or frequencies outside that band. Sections 31–38 instead estimate the entire cosine distribution directly.

31. A fixed spatial region after dilation

We prove (B16) using a finite reflected wave construction with its actual smooth error and the joint no-return kernel estimate, equation (T194). All constants may depend on the fixed operator, dimension and finitely many coefficient bounds.

Use boundary normal coordinates, and represent half densities by their coefficients relative to the coordinate half density. After a constant tangential linear change at a boundary point y0y_0, the principal matrix at that point is the identity. These changes can be chosen smoothly on finitely many boundary patches: the positive matrix square root follows, for example, by the uniformly convergent power series for (I−B)1/2(I-B)^{1/2}, after a fixed positive scalar rescaling makes ∥B∥<1\|B\|<1. Its differentiated series converge on the same compact spectral interval. Put z=(z′,zn)z=(z',z_n), with wall zn=0z_n=0, and dilate the original coordinates about y0y_0 by ε\varepsilon. The resulting differential operator, multiplied by ε2\varepsilon^2, has the form Pε=−∂i(Aεij∂j)+bεi∂i+cε,Aεnn=1,Aεin=0 (i<n),A0=I,b0=0,c0=0,γε(z)=(det⁡Aε(z))−1/2.(B112) \begin{gathered} P_\varepsilon =-\partial_i(A_\varepsilon^{ij}\partial_j) +b_\varepsilon^i\partial_i+c_\varepsilon,\\ A_\varepsilon^{nn}=1,\quad A_\varepsilon^{in}=0\ (i<n),\\ A_0=I,\quad b_0=0,\quad c_0=0,\\ \gamma_\varepsilon(z)=(\det A_\varepsilon(z))^{-1/2}. \end{gathered} \tag{B112} Here bε=O(ε)b_\varepsilon=O(\varepsilon), cε=O(ε2)c_\varepsilon=O(\varepsilon^2), and Aε−I=O(ε)A_\varepsilon-I=O(\varepsilon) on every fixed bounded zz-region, in every fixed derivative norm. The divergence rewriting includes derivatives of the original principal coefficients; no lower-order term is discarded. Parameters y0y_0 are retained throughout.

Fix a scaled time bound T∗=33T_*=33. Take a much larger fixed coordinate ball, with radius exceeding 100(T∗+1)100(T_*+1), and then reduce the permitted ε\varepsilon. The compact extension in (T174)–(T175) works with this radius: increase the tangential periods and normal interval before choosing ε\varepsilon, keep the operator unchanged on that ball, and make it flat outside a slightly larger ball. The same form absorption and fixed-interval Poincaré argument give a common positive Dirichlet realization. All finite elliptic and energy estimates used in (T176) remain uniform. Finite propagation (T157)–(T160), first for smooth data and then for the source limits in (T182)–(T186), identifies its kernel with the physical scaled kernel for the times and points considered here.

Let Π=(0,1)\Pi=(0,1). We need ordinary and once-reflected geodesic coordinates about Π\Pi, also for sources yy in a small fixed neighborhood of Π\Pi. The metric is Aε−1A_\varepsilon^{-1}. Its geodesic equations are the Hamilton equations already constructed by the integral equation in (G13); differentiating that integral equation and applying the elementary integral inequality used there proves smooth dependence on all initial data and parameters on this fixed interval. At ε=0\varepsilon=0, the two endpoint maps, with initial tangent vector SS, are E0(S)=Π+S,E0 r(S)=(S′,−1−Sn),Sn<0.(B113) \begin{gathered} \mathcal E_0(S)=\Pi+S,\\ \mathcal E_0^{\,r}(S)=(S',-1-S_n),\qquad S_n<0. \end{gathered} \tag{B113} The second map continues the incoming ray to the wall and then reverses its normal velocity.

Here are uniform domains for this construction. Take a large fixed R>4(T∗+3)R>4(T_*+3). On ∣S∣<R, Sn<−1/2|S|<R,\ S_n<-1/2, the flat wall-hit parameter is −1/Sn-1/S_n; the angle of incidence is bounded below by 1/(2R)1/(2R). Extend the metric smoothly across the wall for this calculation. The equation for the hit has a uniformly nonzero time derivative, so the proved coordinate inverse lemma gives a smooth hit time for small ε\varepsilon. Reflect the velocity using the metric normal and continue the flow, allowing a negative remaining time when defining the extended endpoint map. Flow estimates make this map and its first derivative uniformly close to (B113). Its derivative stays invertible. More strongly, on this convex SS-domain the fundamental theorem of calculus gives ∣Eε r(S)−Eε r(S~)∣≥12∣S−S~∣.(B114) |\mathcal E_\varepsilon^{\,r}(S) -\mathcal E_\varepsilon^{\,r}(\widetilde S)| \geq \tfrac12|S-\widetilde S|. \tag{B114} Indeed subtract the fixed flat orthogonal linear part and bound the derivative of the difference by 1/21/2. Thus the map is one-to-one. Every retained physical point with ∣z−Π∣≤2T∗+3, zn≥0|z-\Pi|\leq 2T_*+3,\ z_n\geq0 lies in its image: its flat inverse stays a fixed distance from the domain boundary; the map which subtracts the small nonlinear error from this flat inverse is a contraction on a fixed small closed ball. The convergent iteration proves existence, and the inverse lemma proves smoothness. The same argument applies to the ordinary endpoint map on ∣S∣<R|S|<R, and uniformly when yy moves slightly.

All reflected physical segments so obtained occur after the first wall hit. They have no second wall hit in the retained time interval. At the first hit their outward-to-inward reflected normal speed has a fixed positive lower bound; the acceleration is O(ε)O(\varepsilon) on this bounded region. Its total change is smaller than half that bound when ε\varepsilon is small. This argument also shows that no grazing ray is being omitted from the causal region issuing from a source at height near one: any ray reaching the wall within the fixed time has initial normal speed bounded away from zero.

Write Gy=Aε(y)−1G_y=A_\varepsilon(y)^{-1} and r=∣S∣Gyr=|S|_{G_y}. The ordinary and broken geodesic lengths are rr. Both coordinate pullbacks of the metric have the radial identity A(S)GyS=S.(B115) A(S)G_y S=S. \tag{B115} For completeness, differentiate the length of a unit-speed geodesic variation. Integration of the derivative of its kinetic energy leaves only the endpoint scalar products, because the geodesic equation cancels the interior term. For a broken geodesic there is an additional wall term: the difference of the incoming and outgoing momenta paired with the moving wall point. It is zero because that motion is tangent to the wall and the two tangential momenta agree. Consequently the endpoint radial velocity has scalar product with an arbitrary endpoint variation equal to GyS⋅dS/rG_y S\cdot dS/r. This is the metric identity dual to (B115). It proves that identity for both coordinate systems without a separate geometric comparison theorem. At z=y=Πz=y=\Pi, the reflected length is exactly two: the boundary normal line goes down a unit distance and back a unit distance for every ε\varepsilon, and uniqueness in (B114) identifies it with the reflected inverse just constructed.

32. Flat causal distributions from Fourier multipliers

Let L0=∂t2−ΔzL_0=\partial_t^2-\Delta_z. Define distributions EνE_\nu, ν=0,1,…\nu=0,1,\ldots, by their spatial Fourier transforms E^ν(t,ξ)=(−∂λ)ν[H(t)sin⁡(tλ)λ]λ=∣ξ∣2.(B116) \widehat E_\nu(t,\xi) =(-\partial_\lambda)^\nu \left[H(t)\frac{\sin(t\sqrt\lambda)}{\sqrt\lambda}\right] _{\lambda=|\xi|^2}. \tag{B116} The quotient is defined at zero by its power series. The derivatives in (B116) have polynomial bounds in t,ξt,\xi on compact time intervals, so integration against Schwartz functions defines distributions. Differentiation of the scalar equation gives L0E0=δ(0,0),L0Eν=νEν−1(ν≥1),−2∂ziEν=ziEν−1(ν≥1).(B117) \begin{gathered} L_0E_0=\delta_{(0,0)},\\ L_0E_\nu=\nu E_{\nu-1}\quad(\nu\geq1),\\ -2\partial_{z_i}E_\nu=z_iE_{\nu-1}\quad(\nu\geq1). \end{gathered} \tag{B117} For the second identity differentiate the spatial Fourier transform in ξi\xi_i; the factor is 2ξi∂λ2\xi_i\partial_\lambda, with the sign supplied by the alternating derivative. These operations are valid on Schwartz tests. Rotation invariance follows from the same definition.

Each EνE_\nu is supported in t≥∣z∣t\geq |z|. For E0E_0, approximate the initial delta by smooth data supported in a ball of radius tending to zero. The constant-coefficient energy identity (T158), applied on growing bounded balls and with the exterior cone weight, gives support in t≥∣z∣−ηt\geq |z|-\eta. The Fourier formula gives distributional convergence to E0E_0, proving its asserted support. For the induction, convolution of two distributions supported in the forward cone is well-defined: over the inverse image of a compact set under addition, their two time coordinates are nonnegative and bounded, hence both spatial coordinates are bounded. Insert a compact cutoff equal to one there into the tensor-product pairing. Its value is independent of the cutoff; smoothing both factors gives the usual convolution identities in the limit. Then Eν=νE0∗Eν−1E_\nu=\nu E_0*E_{\nu-1}: both sides solve the same forced equation with zero past, as is verified either by (B116) or by the scalar Fourier ordinary differential equation. This proves support by induction.

With s=1+iτs=1+i\tau, the joint Fourier transform of e−tEνe^{-t}E_\nu is ν!(∣ξ∣2+s2)ν+1.(B118) \frac{\nu!}{(|\xi|^2+s^2)^{\nu+1}}. \tag{B118} This follows by integrating the elementary damped sine transform and differentiating in λ\lambda. There is a constant c>0c>0 such that ∣∣ξ∣2+(1+iτ)2∣≥c⟨(τ,ξ)⟩\big||\xi|^2+(1+i\tau)^2\big|\geq c\langle(\tau,\xi)\rangle. If ∣ξ∣≤2(1+∣τ∣)|\xi|\leq2(1+|\tau|), use its imaginary part 2τ2\tau for large ∣τ∣|\tau| and compactness for bounded τ\tau; if ∣ξ∣>2(1+∣τ∣)|\xi|>2(1+|\tau|), use its positive real part. Thus for ν>n+q\nu>n+q, multiplying (B118) by any polynomial of degree at most qq gives an integrable function on R1+n\mathbb R^{1+n}. Fourier inversion proves Eν∈CqE_\nu\in C^q on compact time regions. In particular its derivatives through order qq vanish at t=0t=0, since it vanishes for negative time. Taking ν\nu larger allows any specified finite number of coordinate and parameter derivatives after a smooth pullback.

The even full-time distributions needed for cosine kernels are Cν(t,z)=∂t[Eν(t,z)−Eν(−t,z)],C^ν(t,ξ)=(−∂λ)νcos⁡(tλ)∣λ=∣ξ∣2.(B119) \begin{gathered} C_\nu(t,z)=\partial_t[E_\nu(t,z)-E_\nu(-t,z)],\\ \widehat C_\nu(t,\xi) =(-\partial_\lambda)^\nu\cos(t\sqrt\lambda) \big|_{\lambda=|\xi|^2}. \end{gathered} \tag{B119} They have a well-defined restriction to every fixed zz, including zero. Indeed time testing of the second formula produces a smooth function of ξ\xi decreasing faster than every power, also after multiplication by any fixed power of ξ\xi. At ξ=0\xi=0, smoothness follows from the even Taylor expansion of the cosine transform. Spatial Fourier inversion therefore defines a smooth function of zz with values in time distributions. We write Cν(t,r)C_\nu(t,r) for its value at any vector of length rr. For r>0r>0, cone support gives supp⁡Cν( ⋅ ,r)⊂{∣t∣≥r}.(B120) \operatorname{supp} C_\nu(\,\cdot\,,r) \subset\{|t|\geq r\}. \tag{B120} This definition avoids restricting the individual retarded fundamental solution to its singular vertex.

33. Transport with the complete differential operator

Pull PεP_\varepsilon back by either endpoint map. Rewrite it as P=−div⁡(A∇)+b⋅∇+cP=-\operatorname{div}(A\nabla)+b\cdot\nabla+c in the SS-coordinates. The transformed first-order coefficient includes the coordinate Jacobian terms. The matrix identity (B115) gives div⁡(A∇f(r))=div⁡(Gy−1∇f(r))\operatorname{div}(A\nabla f(r))=\operatorname{div}(G_y^{-1}\nabla f(r)). This follows by substituting ∇f=GySf′(r)/r\nabla f=G_y S f'(r)/r; both vector fields equal Sf′(r)/rS f'(r)/r. It remains valid for radial distributions by smoothing radially and taking limits.

Put h(S)=b(S)⋅GySh(S)=b(S)\cdot G_y S. The product rule and (B117) show that the coefficient of Eν−1(t,r)E_{\nu-1}(t,r) in L(uνEν)L(u_\nu E_\nu), for ν≥1\nu\geq1, is νuν+S⋅∇uν−huν/2\nu u_\nu+S\cdot\nabla u_\nu-hu_\nu/2. The remaining term is (Puν)Eν(Pu_\nu)E_\nu. Choose 2S⋅∇u0−hu0=0,u0(0)=1,(ν+S⋅∇−h/2)uν=−Puν−1,u0(S)=exp⁡ ⁣(12∫01h(aS)a da),uν(S)=−u0(S)∫01aν−1(Puν−1)(aS)u0(aS) da.(B121) \begin{gathered} 2S\cdot\nabla u_0-hu_0=0,\quad u_0(0)=1,\\ (\nu+S\cdot\nabla-h/2)u_\nu=-Pu_{\nu-1},\\ u_0(S)=\exp\!\left(\frac12\int_0^1 \frac{h(aS)}a\,da\right),\\ u_\nu(S)=-u_0(S)\int_0^1 a^{\nu-1}\frac{(Pu_{\nu-1})(aS)}{u_0(aS)}\,da. \end{gathered} \tag{B121} Since h(0)=0h(0)=0, every integrand is smooth at the lower endpoint; the formula for u0u_0 can equally be written using the integral of dhdh along the segment. The displayed integrals and differentiation under them prove smoothness and all finite uniform parameter bounds. Differentiating along a ray verifies the equations. A bounded homogeneous solution of the equation for uν/u0u_\nu/u_0, ν>0\nu>0, is a multiple of r−νr^{-\nu}, so regularity at the origin gives uniqueness.

There is no unaccounted vertex term for ν=0\nu=0. Its cross term is V⋅∇E0V\cdot\nabla E_0, where V=u0b−2A∇u0V=u_0b-2A\nabla u_0; transport says V⋅GyS=0V\cdot G_yS=0. After a constant linear change making Gy=IG_y=I, a smooth tangent vector field satisfies V(0)=0V(0)=0 and can be written Vi(S)=∑jaij(S)Sj,aij=∫01a(∂jVi−∂iVj)(aS) da.(B122) \begin{gathered} V_i(S)=\sum_j a_{ij}(S)S_j,\\ a_{ij}=\int_0^1 a (\partial_jV_i-\partial_iV_j)(aS)\,da. \end{gathered} \tag{B122} To verify this, differentiate S⋅V(S)=0S\cdot V(S)=0, sum over jj, and integrate d[aVi(aS)]/dad[aV_i(aS)]/da. The matrix aija_{ij} is skew. Every resulting angular derivative annihilates the radial distribution E0E_0. This proves the cancellation at the vertex as well as away from it.

For the reflected coefficients vνv_\nu, solve the same transport equations in the reflected coordinates, now prescribing their values on the wall to be the incident coefficients at that same physical point. The wall in each radial direction is r=rb>0r=r_b>0, with rbr_b smooth and uniformly separated from zero on the retained domain. The equation rv0′−hv0/2=0r v_0'-h v_0/2=0 is solved by its integrating factor with the specified boundary value; for ν>0\nu>0, multiply the equation for vν/v0v_\nu/v_0 by rνr^\nu and integrate its known right side from rbr_b to rr. Equivalently one can use the nonvanishing homogeneous integrating factor even when the prescribed v0v_0 is not used as a divisor. Here v0v_0 is nonzero after shrinking ε\varepsilon, since its flat value is one. These explicit one-dimensional integrations prove smoothness, uniqueness and all finite uniform bounds, including the source and ε\varepsilon parameters.

At a wall point the ordinary and reflected lengths agree, and the coefficients were chosen equal. Their difference therefore has zero Dirichlet trace term by term. Telescoping (B121) gives the following finite retarded kernel, relative to Lebesgue measure in the original scaled coordinates: KN(t,z,y)=γε(y)∑ν=0N(Iν−Jν),Iν=uνEν(t,ri),Jν=vνEν(t,rr),(∂t2+Pε,z)KN=δ(t)δy(z)+FN(t,z,y).(B123) \begin{gathered} K_N(t,z,y)=\gamma_\varepsilon(y) \sum_{\nu=0}^N(I_\nu-J_\nu),\\ I_\nu=u_\nu E_\nu(t,r_i),\quad J_\nu=v_\nu E_\nu(t,r_r),\\ (\partial_t^2+P_{\varepsilon,z})K_N\\ =\delta(t)\delta_y(z)+F_N(t,z,y). \end{gathered} \tag{B123} In (B123), the coefficients and lengths in Iν,JνI_\nu,J_\nu are evaluated at (z,y)(z,y). Here FN/γε(y)F_N/\gamma_\varepsilon(y) is (PεuN)EN(t,ri)−(PεvN)EN(t,rr)(P_\varepsilon u_N)E_N(t,r_i) -(P_\varepsilon v_N)E_N(t,r_r). The factor γε(y)\gamma_\varepsilon(y) is essential: the constant-metric radial fundamental solution has source (det⁡Aε(y))1/2δy(\det A_\varepsilon(y))^{1/2}\delta_y. This follows by the linear substitution S=Aε(y)1/2wS=A_\varepsilon(y)^{1/2}w; the ordinary endpoint map has derivative the identity at the source. Multiplication by γε(y)\gamma_\varepsilon(y) gives exactly the unit delta in (B123).

For ε=0\varepsilon=0, both pulled-back operators are −Δ-\Delta. Consequently u0=v0=1u_0=v_0=1 and uν=vν=0u_\nu=v_\nu=0 for ν≥1\nu\geq1. Smooth dependence and the fundamental theorem of calculus give, at the diagonal z=y=Πz=y=\Pi, u0(Π,Π)=1,ri(Π,Π)=0,rr(Π,Π)=2,∣v0(Π,Π)−1∣≤Cε,∣uν(Π,Π)∣+∣vν(Π,Π)∣≤Cνε(ν≥1).(B124) \begin{gathered} u_0(\Pi,\Pi)=1,\quad r_i(\Pi,\Pi)=0,\\ r_r(\Pi,\Pi)=2,\quad |v_0(\Pi,\Pi)-1|\leq C\varepsilon,\\ |u_\nu(\Pi,\Pi)|+|v_\nu(\Pi,\Pi)| \leq C_\nu\varepsilon\quad(\nu\geq1). \end{gathered} \tag{B124} These bounds retain every lower-order coefficient.

34. The smooth error is an error for the actual kernel

Choose a spatial cutoff equal to one on the entire causal region from the source neighborhood for 0≤t≤T∗0\leq t\leq T_*, supported inside the larger region of Section 31. Such a cutoff can be chosen independently of the parameters. Indeed the metric is uniformly close to the identity, so a path of length at most T∗+1T_*+1 stays in ∣z−Π∣<2T∗+3|z-\Pi|<2T_*+3. Put the cutoff transition farther away. On its transition, both terms of (B123) vanish by cone support throughout the retained time interval. Multiplying the parametrix by this cutoff introduces no forcing there. It also preserves the exact wall cancellation. The construction now extends by zero to the fixed compact extension.

For any prescribed finite integer qq, choose NN sufficiently large in (B118). The residual is jointly CqC^q in time, target, source and the retained parameters, vanishes to as many prescribed orders at t=0t=0 as needed, and obeys ∥FN∥Cq([0,T∗]×X×Y)≤Cqε.(B125) \|F_N\|_{C^q([0,T_*]\times X\times Y)} \leq C_q\varepsilon. \tag{B125} The same statement holds with any specified finite list of derivatives in y0y_0 and one derivative in ε\varepsilon before taking the final O(ε)O(\varepsilon) difference. To justify it at the incident vertex, work in the smooth vector coordinate SS, where EN(t,∣S∣Gy)E_N(t,|S|_{G_y}) is a Cq′C^{q'} function for a larger chosen q′q'. The radial square root need not be differentiated at S=0S=0. Every coefficient and map is smooth on the fixed compact region. At ε=0\varepsilon=0, FN=0F_N=0; integrate its uniformly bounded ε\varepsilon-derivative.

We give the finite regularity estimate that turns (B125) into an actual kernel error. If (∂t2+Pε)V=F,V∣∂X=0,V(0)=Vt(0)=0.(B126) \begin{gathered} (\partial_t^2+P_\varepsilon)V=F,\\ V|_{\partial X}=0,\quad V(0)=V_t(0)=0. \end{gathered} \tag{B126} then a sufficiently large finite collection of ordinary derivatives of a smooth FF, vanishing to sufficiently high time order at zero, bounds any specified CrC^r norm of VV. All constants are uniform in this compact coefficient family.

Here are the details of the estimate. The full-coefficient energy inequality (T158), or its unweighted case integrated in time, bounds ∥Vt(t)∥2+∥V(t)∥H1\|V_t(t)\|_2+\|V(t)\|_{H^1} by C∫0t∥F(s)∥2 dsC\int_0^t\|F(s)\|_2\,ds. Apply it to ∂tjV\partial_t^jV. Differentiating the equation at zero shows that its two initial values are zero as long as the corresponding derivatives of FF vanish there. Thus any specified finite number of time derivatives is bounded in H1H^1. The smooth Dirichlet reading, Theorem 3.1, equation (16), with the uniform-constant argument in (T176), gives, for integers a≥0a\geq0, ∥∂tjV∥Ha+2≤Ca(∥∂tjF∥Ha+∥∂tj+2V∥Ha+∥∂tjV∥2).(B127) \begin{gathered} \|\partial_t^jV\|_{H^{a+2}}\\ \leq C_a\bigl( \|\partial_t^jF\|_{H^a} +\|\partial_t^{j+2}V\|_{H^a}\\ \qquad{}+\|\partial_t^jV\|_2\bigr). \end{gathered} \tag{B127} Starting with the time-energy bounds and descending through a sufficiently long finite list of time derivatives proves this estimate successively for every needed spatial order. Smooth approximation of FF, the energy difference estimate and the elliptic estimate justify the induction for the solution defined by the spectral sine propagator. Sobolev embedding, proved by the Fourier extension argument in the same reading, then bounds the requested ordinary derivatives up to the wall.

Source derivatives commute with (B126) and differentiate FF only. A coefficient-parameter derivative satisfies the same equation with forcing ∂ωF−(∂ωPε)V\partial_\omega F-(\partial_\omega P_\varepsilon)V. The second term uses at most two additional spatial derivatives of the already bounded VV. Induction on the desired finite number of parameter derivatives, choosing two more spatial orders at each such step, proves the claimed uniform estimate. This argument uses only the common first Dirichlet domain and ordinary boundary elliptic estimates; it does not differentiate a parameter-dependent higher power domain. In particular (B125) bounds the solution and its first time derivative, jointly at target and source, by CεC\varepsilon.

The actual retarded sine kernel minus KNK_N is the solution of (B126) with forcing −FN-F_N. One can verify the identification without assuming pointwise convergence of a wave series. Test first against a smooth source function supported near Π\Pi. The source and boundary terms in (B123) are exact, so subtraction has zero past and the smooth forcing just described. Uniqueness follows by testing the homogeneous difference against Dirichlet eigensections: its scalar coefficients solve vj′′+λjvj=0v_j''+\lambda_jv_j=0 with zero past and hence vanish. Distributional testing is legitimate after time smoothing; the zero boundary trace removes the boundary term, and the resulting finite-order distributions are recovered by removing the smoothing. Completeness of the smooth spectral tests, equivalently inverse-power regularization (W9)–(W12), gives zero difference. Differentiation in the smooth source parameter followed by testing identifies the jointly smooth error kernel. Thus this is an equality of the actual kernels.

Write aν=uν(Π,Π)a_\nu=u_\nu(\Pi,\Pi) and bν=vν(Π,Π)b_\nu=v_\nu(\Pi,\Pi). Taking the odd-time difference and one time derivative, and converting the diagonal from Lebesgue measure to metric volume, gives Cε(t):=γε(Π)−1CPε(t,Π,Π),Cε(t)=C0(t,0)−b0C0(t,2)+∑ν=1NaνCν(t,0)−∑ν=1NbνCν(t,2)+Rε(t),∥Rε∥C0([−32,32])≤Cε.(B128) \begin{gathered} \mathcal C_\varepsilon(t) :=\gamma_\varepsilon(\Pi)^{-1} C_{P_\varepsilon}(t,\Pi,\Pi),\\ \mathcal C_\varepsilon(t)=C_0(t,0)-b_0 C_0(t,2)\\ \quad+\sum_{\nu=1}^N a_\nu C_\nu(t,0)\\ \quad-\sum_{\nu=1}^N b_\nu C_\nu(t,2)+R_\varepsilon(t),\\ \|R_\varepsilon\|_{C^0([-32,32])}\leq C\varepsilon. \end{gathered} \tag{B128} For any fixed greater regularity of the remainder, increase NN. The γε(y)\gamma_\varepsilon(y) in (B123) cancels exactly with the diagonal conversion 1/γε(Π)1/\gamma_\varepsilon(\Pi). The coefficient of C0(t,0)C_0(t,0) is exactly one. Restrictions at that term are the time-tested restrictions from (B119); the smooth remainder supplies the same restriction for the actual kernel. This proves both the normalization and the actual finite remainder.

35. Coarse temporal estimates, including the singular vertex

We require only polynomial bounds, not a stationary-phase expansion. Introduce the mass parameter m≥0m\geq0: C[m](t,z)=(2π)−n∫eiz⋅ξcos⁡(t∣ξ∣2+m) dξ.(B129) \begin{gathered} C^{[m]}(t,z)\\ =(2\pi)^{-n}\int e^{iz\cdot\xi} \cos(t\sqrt{|\xi|^2+m})\,d\xi . \end{gathered} \tag{B129} All integrals here are time-tested distributions. The even Taylor expansion at frequency zero and rapid decay at infinity justify every right derivative at m=0m=0, giving Cν=(−∂m)νC[m]∣m=0C_\nu=(-\partial_m)^\nu C^{[m]}|_{m=0}. For ∣τ∣≥1|\tau|\geq1 and 0≤m<1/40\leq m<1/4, polar integration gives its time Fourier transform: FtC[m](τ,z)=π(2π)−n∣τ∣(τ2−m)(n−2)/2⋅∫Sn−1eiτ2−m z⋅ω dω.(B130) \begin{gathered} \mathcal F_t C^{[m]}(\tau,z) =\pi(2\pi)^{-n}|\tau|(\tau^2-m)^{(n-2)/2}\\ \qquad\cdot\int_{S^{n-1}} e^{i\sqrt{\tau^2-m}\,z\cdot\omega}\,d\omega . \end{gathered} \tag{B130} Indeed the transform of the cosine is π[δ(τ−r2+m)+δ(τ+r2+m)]\pi[\delta(\tau-\sqrt{r^2+m})+\delta(\tau+\sqrt{r^2+m})]. The radial Jacobian is ∣τ∣/r|\tau|/r, which, multiplied by rn−1r^{n-1}, gives the displayed power. This proves every constant in (B130).

At ∣z∣=2|z|=2, differentiating the amplitude and exponential any fixed number of times in mm gives the bound Cν⟨τ⟩n−1C_\nu\langle\tau\rangle^{n-1}; each derivative of the square root introduces a bounded inverse power when ∣τ∣≥1|\tau|\geq1. At z=0z=0 and ν≥1\nu\geq1, the sphere integral is constant and the bound improves to Cν⟨τ⟩n−1−2νC_\nu\langle\tau\rangle^{n-1-2\nu}, hence to Cν⟨τ⟩n−2C_\nu\langle\tau\rangle^{n-2}. The part in ∣τ∣≤2|\tau|\leq2 is a compactly supported distribution of finite order by (B119). Convolution with the Fourier transform of a compact smooth time cutoff makes that part rapidly decreasing: apply its finite-order test bound to the translated Schwartz function. Convolution of the high-frequency part with a Schwartz function preserves either of the nonnegative power bounds just given, by ⟨τ−σ⟩a≤Ca⟨τ⟩a⟨σ⟩a\langle\tau-\sigma\rangle^a\leq C_a\langle\tau\rangle^a\langle\sigma\rangle^a.

Let ψ\psi range over a bounded set in Cc∞((−32,32))C_c^\infty((-32,32)). We obtain, for κ≥0\kappa\geq0, ∣⟨Cν(t,2),ψ(t)sin⁡(κt)t⟩∣≤Cνκ(1+κ)n−2,∣⟨Cν(t,0),ψ(t)sin⁡(κt)t⟩∣≤Cνκ(1+κ)n−2,ν≥1.(B131) \begin{gathered} \left|\left\langle C_\nu(t,2), \psi(t)\frac{\sin(\kappa t)}t\right\rangle\right|\\ \leq C_\nu\kappa(1+\kappa)^{n-2},\\ \left|\left\langle C_\nu(t,0), \psi(t)\frac{\sin(\kappa t)}t\right\rangle\right|\\ \leq C_\nu\kappa(1+\kappa)^{n-2}, \quad \nu\geq1. \end{gathered} \tag{B131} For the first line insert a smooth cutoff vanishing near zero and equal to one on ∣t∣≥2|t|\geq2; (B120) allows this without change. Then ψ(t)/t\psi(t)/t is an ordinary compact smooth test coefficient. Its Fourier convolution is bounded by C(1+κ)n−1C(1+\kappa)^{n-1} for κ≥1\kappa\geq1, which is comparable to the stated bound. For 0≤κ≤10\leq\kappa\leq1, the test function and all needed derivatives are O(κ)O(\kappa); use the finite distribution order.

For the second line denote the pairing by Jν(κ)J_\nu(\kappa). It is zero at κ=0\kappa=0, and differentiation under distributional pairing gives Jν′(κ)=⟨Cν(t,0),ψ(t)cos⁡(κt)⟩J_\nu'(\kappa)=\langle C_\nu(t,0),\psi(t)\cos(\kappa t)\rangle. The improved high-frequency bound just proved and its low-frequency part bound this derivative by C(1+κ)n−2C(1+\kappa)^{n-2}. Integration from zero proves (B131). This argument works also when n=2n=2, including any point-supported terms at zero temporal frequency.

For a bounded ordinary function RR on this fixed interval, ∣∫R(t)ψ(t)sin⁡(κt)t dt∣≤C∥R∥∞κ.(B132) \left|\int R(t)\psi(t) \frac{\sin(\kappa t)}t\,dt\right| \leq C\|R\|_\infty\kappa. \tag{B132} This is simply ∣sin⁡(κt)/t∣≤κ|\sin(\kappa t)/t|\leq\kappa and the finite interval length.

36. The reflected-arrival part of the actual comparison

Choose an even smooth χ\chi, equal to one on [−16,16][-16,16] and supported in (−32,32)(-32,32). The physical diagonal is at distance dd; set ε=d\varepsilon=d, t=dut=du, and κ=kd\kappa=kd. Unitary spatial dilation of the coordinate half densities multiplies a kernel by d−nd^{-n}. Conversion to metric volume then gives the exact distributional identity Cx(du)=d−nCd(u),Cd0(du)=d−n[C0(u,0)−C0(u,2)].(B133) \begin{gathered} C_x(du)=d^{-n}\mathcal C_d(u),\\ C_d^0(du)=d^{-n}[C_0(u,0)-C_0(u,2)]. \end{gathered} \tag{B133} These identities mean pullback under the nonzero linear time dilation; on pairing, the time Jacobian dd is retained. It cancels the factor dd in the denominator of sin⁡(kt)/t\sin(kt)/t.

The test coefficients ψd(u)=χ(u)ρ^(du)\psi_d(u)=\chi(u)\widehat\rho(du) form a bounded set of compact smooth functions. Subtract the two identities in (B133), insert (B128), and use (B124), (B131), (B132). The direct leading term cancels exactly. The reflected leading coefficient differs by O(d)O(d), and all higher coefficients and the smooth error are O(d)O(d). Therefore ∣⟨Cx−Cd0,χ(t/d)ρ^(t)sin⁡(kt)t⟩∣≤Cd1−nκ(1+κ)n−2=Ck(k+d−1)n−2.(B134) \begin{gathered} \left|\left\langle C_x-C_d^0, \chi(t/d)\widehat\rho(t)\frac{\sin(kt)}t \right\rangle\right|\\ \leq C d^{1-n}\kappa(1+\kappa)^{n-2} =C k(k+d^{-1})^{n-2}. \end{gathered} \tag{B134} There is no lower-energy cutoff in this calculation; it bounds the complete short-time cosine distribution.

37. The part with time much larger than distance

For 16d≤∣t∣≤T16d\leq |t|\leq T, put ε=∣t∣\varepsilon=|t| and θ=d/∣t∣≤1/16\theta=d/|t|\leq1/16. Let zθ=(0,θ)z_\theta=(0,\theta). The coordinate and density scaling used in (B133), now at time scale ε\varepsilon, gives Cx(t)=∣t∣−nγε(zθ)−1CPε(1,zθ,zθ).(B135) C_x(t)=|t|^{-n} \gamma_\varepsilon(z_\theta)^{-1} C_{P_\varepsilon}(1,z_\theta,z_\theta). \tag{B135} Evenness of the cosine kernel handles negative time. Choose the physical TT small enough that these scaled families fall within (T174)–(T194). The latter theorem says that the right-hand kernel at time one is smooth with every parameter, source and target derivative, uniformly for 0≤θ≤1/160\leq\theta\leq1/16 and 0≤ε≤T0\leq\varepsilon\leq T.

Denote the normalized kernel in (B135) by F(ε,y0,θ)F(\varepsilon,y_0,\theta). At ε=0\varepsilon=0, the operator is the flat half-space operator throughout the domain of dependence, so the odd Fourier calculation gives F(0,y0,θ)=C0(1,0)−C0(1,2θ)F(0,y_0,\theta)=C_0(1,0)-C_0(1,2\theta). These are smooth values since 1>2θ1>2\theta. At θ=0\theta=0, both source and target are at the Dirichlet wall, so F(ε,y0,0)=0F(\varepsilon,y_0,0)=0. The limiting source assertion follows explicitly from the boundary source limits in (T182)–(T186). Set G=F−[C0(1,0)−C0(1,2θ)]G=F-[C_0(1,0)-C_0(1,2\theta)]. It vanishes on both parameter axes. The twice iterated fundamental theorem of calculus gives G(ε,y0,θ)=∫0ε∫0θ∂a∂bG(a,y0,b) db da,∣Cx(t)−Cd0(t)∣≤Cd ∣t∣−n,16d≤∣t∣≤T.(B136) \begin{gathered} G(\varepsilon,y_0,\theta)\\ =\int_0^\varepsilon\int_0^\theta \partial_a\partial_bG(a,y_0,b)\,db\,da,\\ |C_x(t)-C_d^0(t)|\leq C d\,|t|^{-n},\\ 16d\leq|t|\leq T. \end{gathered} \tag{B136} The mixed derivative is bounded by the actual kernel theorem (T194), including the zero scaling endpoint; this is where its parameter assertion is used.

Pair this smooth function with the complementary time cutoff. The two elementary inequalities ∣sin⁡(kt)∣≤k∣t∣|\sin(kt)|\leq k|t| and ∣sin⁡(kt)∣≤1|\sin(kt)|\leq1 give ∣⟨Cx−Cd0,[1−χ(t/d)]ρ^(t)sin⁡(kt)t⟩∣≤Cmin⁡{kd2−n, d1−n}=Cd1−nmin⁡{kd,1}≤Ck(k+d−1)n−2.(B137) \begin{gathered} \left|\left\langle C_x-C_d^0, [1-\chi(t/d)]\widehat\rho(t)\frac{\sin(kt)}t \right\rangle\right|\\ \leq C\min\{k d^{2-n},\,d^{1-n}\}\\ =C d^{1-n}\min\{kd,1\}\\ \leq C k(k+d^{-1})^{n-2}. \end{gathered} \tag{B137} For example the first bound is Ckd∫16dTt−n dtCkd\int_{16d}^T t^{-n}\,dt, and the second is Cd∫16dTt−n−1 dtCd\int_{16d}^T t^{-n-1}\,dt. Both integrals have the stated bounds for n≥2n\geq2. If 16d≥T16d\geq T, this part is empty. Thus no small-distance or energy range is left out.

38. Completion of the curved spectral estimate

Adding (B134) and (B137), and reinstating the harmless factor 1/π1/\pi, proves (B16) for a fixed collar 0<d≤d00<d\leq d_0. The two tails in (B13) then prove (B7). The positive unsmoothing proof in Section 3 gives, for k≥2k\geq2, eP(x,x;k2)=kn[Wn(0)−Wn(2kd(x))]+R(x,k),∣R(x,k)∣≤Ckn,∣R(x,k)∣≤Ck(k+d(x)−1)n−2,d(x)>0.(B138) \begin{gathered} e_P(x,x;k^2)\\ =k^n[W_n(0)-W_n(2kd(x))]+R(x,k),\\ |R(x,k)|\leq C k^n,\\ |R(x,k)|\leq C k(k+d(x)^{-1})^{n-2},\\ d(x)>0. \end{gathered} \tag{B138} Here the spectral density is relative to dVgdV_g, and either strict or closed endpoint convention is allowed. At the wall the density, the model and the remainder are all zero.

For use beyond the small collar, the same proof also supplies the requisite interior estimate. On the compact region d(x)≥d0d(x)\geq d_0, take one fixed time smaller than the boundary distance and a uniform geodesic coordinate radius. Repeat Sections 31–34 with the ordinary endpoint map alone, without dilation. The coefficients uν(x,x)u_\nu(x,x) and the smooth error are uniformly bounded, and u0(x,x)=1u_0(x,x)=1. The same source normalization cancels against metric volume. Applying the second line of (B131) and (B132) therefore bounds the smoothed difference from the bulk model (2π)−nωnkn(2\pi)^{-n}\omega_n k^n by Ckn−1Ck^{n-1}. The positive argument of Section 3, now with weight (1+∣k∣)n−1(1+|k|)^{n-1}, gives ∣eP(x,x;k2)−Wn(0)kn∣≤Ckn−1,d(x)≥d0.(B139) \begin{gathered} \left|e_P(x,x;k^2)-W_n(0)k^n\right| \leq C k^{n-1},\\ d(x)\geq d_0. \end{gathered} \tag{B139} All steps in that argument remain unchanged: the bulk model has positive derivative bounded by Ckn−1Ck^{n-1}, the fixed smoothing is positive, and the actual rough growth is (B1).

Finally ∣Wn(s)∣≤C/(1+s)|W_n(s)|\leq C/(1+s) for s≥0s\geq0. For s≥1s\geq1, slice the unit ball in its last coordinate. The remaining amplitude is a constant times (1−a2)(n−1)/2(1-a^2)^{(n-1)/2} on [−1,1][-1,1]; it is zero at the endpoints and has integrable derivative for every n≥2n\geq2. One integration by parts bounds its Fourier integral by C/sC/s. For s≤1s\leq1, use the volume bound. Hence kn∣Wn(2kd)∣≤Cd0kn−1k^n|W_n(2kd)|\leq C_{d_0}k^{n-1} when d≥d0d\geq d_0. Combining this with (B139) proves (B138) throughout XX, without assuming that the distance function is smooth outside the collar.

Estimate (B138) holds for the full scalar, smooth, formally self-adjoint, strictly positive Dirichlet operator stated at the start, including all lower-order terms. It supplies the two bounds in the integrated remainder transfer theorem and the pointwise input in Generalized rays and the Dirichlet Weyl law.

Victor Ivrii's freely readable author monograph, Microlocal Analysis, Sharp Spectral Asymptotics and Applications, July 9, 2023 version, Section 8.1.2, printed pp. 741–749, distinguishes boundary parametrices, Tauberian comparison and coefficient freezing. Propositions 8.1.3–8.1.5 lead to Theorem 8.1.6. Section 8.1.1 identifies a tangential energy direction away from normal incidence; the pointwise complementary route uses Theorem 7.3.2 with Remark 7.3.3(v), supported by Theorem 7.2.17(i). Sections 5–30 above develop the near-normal and frozen parts of that route explicitly.

For the construction in Sections 31–38, see also Lars Hörmander, The Analysis of Linear Partial Differential Operators III: Pseudo-Differential Operators, the 2007 electronic edition. Section 17.4, printed pp. 32–40, constructs ordinary and reflected radial wave parametrices; Proposition 17.4.4 identifies their finite residual. Theorem 17.5.10, printed p. 52, is the corresponding curved spectral estimate.

The two-scale comparison uses the joint parameter kernel theorem, including boundary source limits. The Fourier distributions and radial transports in Sections 32–34 control the reflected arrival; the uniform kernel theorem controls later times. Section 3 then removes the positive smoothing.

The near-normal and complementary frozen calculations in Sections 5–30 provide more detailed descriptions of the corresponding localized models.