Reading settings

Settings and reading history are stored only in this browser.

English中文0%

Select a passage or formula to leave a suggestion here. Saved suggestions remain private until reviewed.

Appendix: three-variable chart calculations

This appendix concerns Definition 4.1 and Lemmas 4.2–4.4 on pp. 15–20 of H, and proves only the forms needed for the fixed-triple scale estimate. We denote the number of spatial variables by s∈{1,2,3}s\in\{1,2,3\} to distinguish it from the accuracy parameter kk in the main text.

1. Charts, translations, and quantitative dependence

Write e(t)=exp⁡(2πit)\mathrm e(t)=\exp(2\pi it). Consider

Q(z)=e(zTΛz+bTz)∑n∈Zdχ(Vz−n)e((Vz)TC(Vz−n)),z∈Rs, Q(z)=\mathrm e(z^T\Lambda z+b^Tz) \sum_{n\in\mathbb Z^d}\chi(Vz-n) \mathrm e\bigl((Vz)^TC(Vz-n)\bigr),\quad z\in\mathbb R^s,

where Λ\Lambda is symmetric, VV and bb are an arbitrary real matrix and vector, and CC is a rational matrix. Complexity H≥e2H\ge\mathrm e^2 means

d≤log⁡H,ht⁡(C)≤H,supp⁡χ⊂[−H,H]d, d\le\log H,\quad\operatorname{ht}(C)\le H, \quad\operatorname{supp}\chi\subset[-H,H]^d,
∥∂αχ∥∞≤Hc0(∣α∣+1)(∣α∣+1)c0(∣α∣+1). \|\partial^\alpha\chi\|_\infty \le H^{c_0(|\alpha|+1)}(|\alpha|+1)^{c_0(|\alpha|+1)}.

The fixed-order Gevrey constant c0c_0 does not change with any real frequency. At each point there are at most (2H+3)d(2H+3)^d nonzero lattice terms, so the absolute value of QQ has a quasipolynomial upper bound in HH. No control of V,Λ,bV,\Lambda,b is needed.

Conjugation, products of a fixed number of factors, and affine substitutions preserve this form. Translation deserves an explicit calculation. Choose an integer PP such that PCPC is an integer matrix; we may take P≤Hd2P\le H^{d^2}. For a horizontal shift aa, write

a=m0+a0,m0∈PZd,∥a0∥∞≤P. a=m_0+a_0,\quad m_0\in P\mathbb Z^d, \quad\|a_0\|_\infty\le P.

Relabel the lattice points and set u=Vz,w=u−nu=Vz,w=u-n. Modulo integers,

(u+m0+a0)TC(w+a0)=uTCw+uTCa0+m0TCu+a0TC(w+a0)+m0TCa0. \begin{aligned} (u+m_0+a_0)^TC(w+a_0) ={}&u^TCw+u^TCa_0+m_0^TCu\\ &+a_0^TC(w+a_0)+m_0^TCa_0. \end{aligned}

The last term is constant. The two middle terms enter the unrestricted ordinary linear phase, and the small-shift term involving ww is absorbed into the smooth amplitude. The support and derivatives of the amplitude depend only on the bounded a0a_0, not on the possibly large m0m_0. Translating the ordinary quadratic phase changes only its linear and constant terms. Thus, after recentering at a fixed path point yy, the complexity remains uniform, and all new real parameters are fixed along that path.

Below, D1,D2,…D_1,D_2,\ldots denote quasipolynomial quantities in HH and the reciprocal of the current threshold. Only a fixed number of such enlargements are made at each step.

2. A large Fourier value controls every small return

Let ϑ\vartheta be supported in a fixed box, with absolute value and Lipschitz norm at most HH. Suppose

F=ϑQ,0<γ<1/2,sup⁡ξ∣F^(ξ)∣≥γ. F=\vartheta Q,\quad 0<\gamma<1/2, \quad\sup_\xi|\widehat F(\xi)|\ge\gamma.

The Fourier transform uses the exponential e(−ξ⋅z)\mathrm e(-\xi\cdot z). We may choose a uniform D1D_1 such that

∥F∥2≤D1,∫(1+∥z∥)∣F(z)∣ dz≤D1, \|F\|_2\le D_1, \quad\int(1+\|z\|)|F(z)|\,\mathrm dz\le D_1,

and such that F^\widehat F is D1D_1-Lipschitz.

Write

A=C−CT,Csy=C+CT2,Csk=C−CT2,sym⁡(B)=B+BT2. A=C-C^T,\quad C_{\mathrm{sy}}=\frac{C+C^T}{2},\quad C_{\mathrm{sk}}=\frac{C-C^T}{2},\quad \operatorname{sym}(B)=\frac{B+B^T}{2}.

The last definition applies to any square matrix BB. For any return

Vh=m+dh,m∈PZd, Vh=m+d_h,\quad m\in P\mathbb Z^d,

translate the variable and relabel the lattice points by n+mn+m. This yields

F(z+h)=e(c(h,m))e(Ω(h,m)⋅z)F(z)+Eh,m(z), F(z+h)=\mathrm e(c(h,m))\mathrm e(\Omega(h,m)\cdot z)F(z)+E_{h,m}(z),
Ω(h,m)=(2Λ+VTCV)h−VTAm,∥Eh,m∥1≤D1(∥h∥+∥dh∥)(return identity) \Omega(h,m)=(2\Lambda+V^TCV)h-V^TAm, \quad \|E_{h,m}\|_1\le D_1(\|h\|+\|d_h\|) \tag{return identity}

whenever the parenthesized quantity on the right is at most 11.

No error depending on VV is hidden here. Set u=Vz,w=u−n,d=dhu=Vz,w=u-n,d=d_h. The nonconstant increment of the chart phase is

uTCd+mTCu+dTCw. u^TCd+m^TCu+d^TCw.

The first two terms equal

zT(VTCVh−VTAm), z^T(V^TCVh-V^TAm),

The last term contains only ww, bounded on the amplitude support, and the small quantity dd. The discarded mTCnm^TCn is an integer. The ordinary quadratic phase contributes 2Λh2\Lambda h, while the increment of the ordinary linear phase is constant. Errors from translating the amplitude and ϑ\vartheta are controlled by the same right side.

Choose ξ0\xi_0 with ∣F^(ξ0)∣≥3γ/4|\widehat F(\xi_0)|\ge3\gamma/4, and set

ρ=γ100D1. \rho=\frac{\gamma}{100D_1}.

Take the integer

N=⌈CsD12γ−2ρ−s⌉, N=\left\lceil C_sD_1^2\gamma^{-2}\rho^{-s}\right\rceil,

where CsC_s is sufficiently large to include the volume constants of unit balls in dimensions at most three. Then set

a=min⁡{γ100D1N,1100(1+∥A∥)}. a=\min\left\{\frac{\gamma}{100D_1N}, \frac1{100(1+\|A\|)}\right\}.

If the return satisfies ∥h∥+∥dh∥≤a\|h\|+\|d_h\|\le a, then for every 1≤j≤N1\le j\le N we may apply the return identity to (jh,jm)(jh,jm). Consequently, the absolute values of the Fourier transform satisfy

∣F^(ξ0−jΩ(h,m))∣≥γ/2. |\widehat F(\xi_0-j\Omega(h,m))|\ge\gamma/2.

If ∥Ω(h,m)∥≥1\|\Omega(h,m)\|\ge1, the balls of radius ρ\rho around these points are disjoint. The Lipschitz bound implies ∣F^∣≥γ/3|\widehat F|\ge\gamma/3 on each ball. Plancherel then yields

∥F∥22≥csNρsγ2>D12, \|F\|_2^2\ge c_sN\rho^s\gamma^2>D_1^2,

a contradiction. Thus every sufficiently small return satisfies

∥Ω(h,m)∥<1.(bound for all small returns) \|\Omega(h,m)\|<1. \tag{bound for all small returns}

The reciprocals of all the chosen small quantities remain quasipolynomial in H,γ−1H,\gamma^{-1}. We have not assumed that the Fourier supremum is attained.

3. Constructing a rational fast space from small returns

For two small returns, direct expansion yields

h′TΩ(h,m)−hTΩ(h′,m′)=dh′TAdh−m′TAm. h'^T\Omega(h,m)-h^T\Omega(h',m') =d_{h'}^TAd_h-m'^TAm.

By the explicit choice of aa above,

∣m′TAm∣≤2a+∥A∥a2<1. |m'^TAm|\le2a+\|A\|a^2<1.

The pairing on the left is an integer, so it is zero.

First suppose d≥1d\ge1. Define the centrally symmetric convex body

K=P−1V[−1,1]s+[−1,1]d. \mathcal K=P^{-1}V[-1,1]^s+[-1,1]^d.

It contains the cube and has nonempty interior. Let λi\lambda_i and μi\mu_i be the successive minima of K\mathcal K and K∘\mathcal K^\circ, respectively, with respect to the integer lattice. The required transference bound is

1≤λiμd+1−i≤(d!)2.(polar transference bound) 1\le\lambda_i\mu_{d+1-i}\le(d!)^2. \tag{polar transference bound}

For the lower bound, two linearly independent families of integer vectors whose dimensions sum to d+1d+1 must have a nonzero integer pairing between them. Apply the polar-body inequality.

The upper bound needs only the upper half of Minkowski's second theorem. Its precise statement appears in Martin Henk, Successive Minima and Lattice Points, Theorem 1.3, p. 2:

(∏i=1dλi(B,Γ))vol⁡(B)≤2ddet⁡Γ, \left(\prod_{i=1}^d\lambda_i(B,\Gamma)\right) \operatorname{vol}(B)\le2^d\det\Gamma,

where BB is a centrally symmetric convex body with nonempty interior and Γ\Gamma is a full-rank lattice.

To apply it, choose from K\mathcal K the columns of a matrix TT with largest absolute determinant. Maximality and convexity yield the following inclusions:

TB1d⊂K⊂TB∞d,T−TB1d⊂K∘. TB_1^d\subset\mathcal K\subset TB_\infty^d, \quad T^{-T}B_1^d\subset\mathcal K^\circ.

Therefore

vol⁡(K)vol⁡(K∘)≥4d(d!)2. \operatorname{vol}(\mathcal K)\operatorname{vol}(\mathcal K^\circ) \ge\frac{4^d}{(d!)^2}.

Multiplying the two Minkowski upper bounds yields

∏iλiμi≤(d!)2. \prod_i\lambda_i\mu_i\le(d!)^2.

Every reverse-order product is already at least 11, so each is at most their total product. This proves the transference bound.

Take

L0=16(d!)2,bmax⁡=a100P(d+s+1). L_0=16(d!)^2, \quad b_{\max}=\frac{a}{100P(d+s+1)}.

Among the d+1d+1 half-open intervals

(bmax⁡L0−j−1,bmax⁡L0−j],0≤j≤d, (b_{\max}L_0^{-j-1},b_{\max}L_0^{-j}], \quad 0\le j\le d,

one contains no successive minimum. Denote its left endpoint by b0b_0. Set

U=span⁡(Zd∩b0K). U=\operatorname{span}(\mathbb Z^d\cap b_0\mathcal K).

Every generating integer vector nn can be written as

n=P−1Vh+w,∥h∥∞,∥w∥∞≤b0. n=P^{-1}Vh+w, \quad\|h\|_\infty,\|w\|_\infty\le b_0.

Then m=Pn,dh=−Pwm=Pn,d_h=-Pw defines a small return within the threshold aa. The integer pairing above is zero, proving

A∣U×U=0.(isotropy of the fast space) A|_{U\times U}=0. \tag{isotropy of the fast space}

The threshold also has an explicit lower bound:

b0−1≤bmax⁡−1L0d+1. b_0^{-1}\le b_{\max}^{-1}L_0^{d+1}.

Since d≤log⁡Hd\le\log H, this reciprocal is still a quasipolynomial quantity of the required type.

Suppose r0=dim⁡U<dr_0=\dim U<d. The empty interval ensures λr0+1>L0b0\lambda_{r_0+1}>L_0b_0. The transference bound provides d−r0d-r_0 independent integer vectors

qν∈(16b0)−1K∘. q_\nu\in(16b_0)^{-1}\mathcal K^\circ.

Their pairings with the short integer vectors generating UU have absolute value less than 11, so the pairings vanish. These vectors therefore span exactly U⊥U^\perp. The definition of the polar body also implies

∥qν∥1≤(16b0)−1,∥qνTV∥1≤P(16b0)−1. \|q_\nu\|_1\le(16b_0)^{-1}, \quad\|q_\nu^TV\|_1\le P(16b_0)^{-1}.

Let SS be the full-row-rank integer matrix with these rows, and define

Ps=ST(SST)−1S,Pf=1−Ps. P_s=S^T(SS^T)^{-1}S, \quad P_f=1-P_s.

The Gram matrix SSTSS^T is an invertible integer matrix with determinant at least 11. Cramer's rule and the bounded integer minors control both the rational height of PsP_s and the size of

Vs=PsV=ST(SST)−1(SV) V_s=P_sV=S^T(SS^T)^{-1}(SV)

All bounds are quasipolynomial. If r0=dr_0=d, simply take Ps=0P_s=0.

4. Controlling the effective quadratic matrix in each of three coordinate directions

Write Vf=PfVV_f=P_fV and define

Λ∗=Λ+12VTCsyV+sym⁡(VfTCskVs). \Lambda_*= \Lambda+\frac12V^TC_{\mathrm{sy}}V+ \operatorname{sym}(V_f^TC_{\mathrm{sk}}V_s).

For each coordinate vector ej∈Rse_j\in\mathbb R^s, sample at equally spaced points in [0,b0][0,b_0] the values

P−1V(tej)(modZd). P^{-1}V(te_j)\pmod{\mathbb Z^d}.

Partition the horizontal torus into cubes of side length at most b0/4b_0/4. With more sample points than cubes, two points lie in the same cube. Their difference yields

h=tjej,b0/N0≤tj≤b0,∥dh∥∞≤Pb0/4,N0≤C(1+4/b0)d. h=t_je_j, \quad b_0/N_0\le t_j\le b_0, \quad\|d_h\|_\infty\le Pb_0/4, \quad N_0\le C(1+4/b_0)^d.

Increase the absolute constant if needed to handle noninteger partition counts. This return still satisfies the threshold aa. Its integer part satisfies P−1m∈b0KP^{-1}m\in b_0\mathcal K, so m∈Um\in U.

Thus

m−Vfh=−Pfdh∈U, m-V_fh=-P_fd_h\in U,

and isotropy removes the fast component:

VTA(m−Vfh)=VsTA(m−Vfh). V^TA(m-V_fh)=V_s^TA(m-V_fh).

The already controlled quantities Vs,A,dhV_s,A,d_h bound this expression quasipolynomially.

The matrix identity is

2Λ+VTCV−VTAVf=2Λ∗+VsTCskVs.(matrix remainder) 2\Lambda+V^TCV-V^TAV_f =2\Lambda_*+V_s^TC_{\mathrm{sk}}V_s. \tag{matrix remainder}

Substituting into the return increment yields

2Λ∗h=Ω(h,m)−VsTCskVsh+VsTA(m−Vfh). 2\Lambda_*h =\Omega(h,m)-V_s^TC_{\mathrm{sk}}V_sh +V_s^TA(m-V_fh).

Every term on the right is controlled. Dividing by tjt_j, which has a quantitative lower bound, controls Λ∗ej\Lambda_*e_j column by column. There are at most three columns, so

∥Vs∥+∥Λ∗∥+ht⁡(Ps)+ht⁡(Pf)≤exp⁡(C(1+log⁡H+log⁡(1/γ))C).(three-variable Weyl output) \|V_s\|+\|\Lambda_*\|+ \operatorname{ht}(P_s)+\operatorname{ht}(P_f) \le\exp\bigl(C(1+\log H+\log(1/\gamma))^C\bigr). \tag{three-variable Weyl output}

When d=0d=0, there is no horizontal matrix or chart lattice. Every sufficiently small hh is a return, and Ω=2Λh\Omega=2\Lambda h. Taking h=aej/2h=ae_j/2 directly controls Λ\Lambda, without introducing a zero-dimensional convex body.

5. Obtaining frequencies of a fixed form after splitting

Now assume only that a rational splitting has been obtained, with its height and the sizes of VsV_s and Λ∗\Lambda_* at most BB. This section no longer uses a large Fourier value.

Set

u=Vz,uf=Pfu,us=Psu,w=u−n. u=Vz,\quad u_f=P_fu,\quad u_s=P_su, \quad w=u-n.

The symmetric part satisfies

uTCsyw=12uTCsyu+12wTCsyw−12nTCsyn. u^TC_{\mathrm{sy}}w =\frac12u^TC_{\mathrm{sy}}u+\frac12w^TC_{\mathrm{sy}}w -\frac12n^TC_{\mathrm{sy}}n.

Isotropy means that the bilinear form defined by CskC_{\mathrm{sk}} vanishes whenever both arguments lie in the fast space, so

uTCskw=ufTCskus−ufTCskPsn+usTCskw. u^TC_{\mathrm{sk}}w =u_f^TC_{\mathrm{sk}}u_s-u_f^TC_{\mathrm{sk}}P_sn +u_s^TC_{\mathrm{sk}}w.

The ordinary quadratic part in the first identity and the first term in the second, together with zTΛzz^T\Lambda z, combine to form zTΛ∗zz^T\Lambda_*z.

Choose an even integer P0P_0 clearing the denominators of CsyC_{\mathrm{sy}}. Then

−12nTCsyn(modZ) -\frac12n^TC_{\mathrm{sy}}n\pmod{\mathbb Z}

depends only on n mod P0Zdn\bmod P_0\mathbb Z^d. Let q0q_0 be a common denominator of PsP_s. On the fixed zz box, us=Vszu_s=V_sz is bounded and ww lies in the amplitude support, so

N=Psn=us−Psw N=P_sn=u_s-P_sw

lies in a bounded box of q0−1Zdq_0^{-1}\mathbb Z^d. There are only quasipolynomially many possible NN and residue classes aa.

Group terms by Psn=NP_sn=N and n≡a(modP0Zd)n\equiv a\pmod{P_0\mathbb Z^d}. Remove the known residue-class constant and the linear phase

−ufTCskN=σNTu,σN=−PfTCskN. -u_f^TC_{\mathrm{sk}}N=\sigma_N^Tu, \quad\sigma_N=-P_f^TC_{\mathrm{sk}}N.

To Fourier expand the remaining amplitude, introduce two independent variables s0,u∈Rds_0,u\in\mathbb R^d. All cutoffs below come from one fixed Gevrey cutoff by coordinate products, translations, and dilations at controlled scales, so they have uniform corresponding Gevrey derivative bounds. Choose η(s0)\eta(s_0) so that on all possible VszV_sz its value is 11, with support in [−Lη,Lη]d[-L_\eta,L_\eta]^d. We may take Lη=4(1+CboxB)L_\eta=4(1+C_{\mathrm{box}}B), where the fixed constant CboxC_{\mathrm{box}} bounds the Euclidean norm on the zz box in use. Choose a smooth function EE such that

E(0)=1,supp⁡E⊂{x:∥x∥∞<1/(3q0)}. E(0)=1, \quad\operatorname{supp}E\subset \{x:\|x\|_\infty<1/(3q_0)\}.

Define

FN,a(s0,u)=η(s0)∑n∈a+P0Zdχ(u−n)E(s0−Ps(u−n)−N)×e(12(u−n)TCsy(u−n)+s0TCsk(u−n)). \begin{aligned} F_{N,a}(s_0,u)=\eta(s_0) \sum_{n\in a+P_0\mathbb Z^d} &\chi(u-n)E\bigl(s_0-P_s(u-n)-N\bigr)\\ &\times\mathrm e\left(\frac12(u-n)^TC_{\mathrm{sy}}(u-n) +s_0^TC_{\mathrm{sk}}(u-n)\right). \end{aligned}

At s0=Psus_0=P_su, the input to the equality cutoff is Psn−NP_sn-N. This is a lattice point with denominator q0q_0, so the cutoff keeps exactly the specified group, not an approximate group.

In uu, this function has period P0P_0. Choose the controlled integer P1=⌈4Lη+2⌉P_1=\lceil4L_\eta+2\rceil. The support of η\eta then lies strictly inside this period box, allowing periodization in the s0s_0 direction. The Fourier modes are

e(pTs0/P1+ℓTu/P0),p,ℓ∈Zd. \mathrm e\bigl(p^Ts_0/P_1+\ell^Tu/P_0\bigr), \quad p,\ell\in\mathbb Z^d.

Substitute s0=Psus_0=P_su and restore the linear phase above to obtain

σ=σN+PsTp/P1+ℓ/P0, \sigma=\sigma_N+P_s^Tp/P_1+\ell/P_0,

Thus we have the exact, absolutely convergent expansion

Q(z)=e(zTΛ∗z+bTz)∑νaνe(σνTVz).(form of expansion frequencies) Q(z)=\mathrm e(z^T\Lambda_*z+b^Tz) \sum_\nu a_\nu\mathrm e(\sigma_\nu^TVz). \tag{form of expansion frequencies}

This explains the form ων=βy+VyTσν\omega_\nu=\beta_y+V_y^T\sigma_\nu in the main text. The remaining real horizontal values enter only through VzVz; they do not become unbounded rational coefficients.

6. Truncation, different splittings, and a fixed rational evaluation family

All cutoff scales, periods, numbers of lattice groups, amplitude supports, and bounded phase coefficients are controlled by a quasipolynomial quantity in H,BH,B, denoted by D2D_2. After normalizing each periodic variable to period one, the product and chain rules yield

∥∂αFN,a∥∞≤D2C(∣α∣+d+1)(∣α∣+1)C(∣α∣+1). \|\partial^\alpha F_{N,a}\|_\infty \le D_2^{C(|\alpha|+d+1)} (|\alpha|+1)^{C(|\alpha|+1)}.

This bound does not involve the unbounded fast part of VV. The differentiation variables are s0,us_0,u; we have not differentiated the composition with VzVz.

For a nonzero Fourier index v=(p,ℓ)∈Z2dv=(p,\ell)\in\mathbb Z^{2d}, choose its coordinate with largest absolute value and integrate by parts mm times. This yields

∣F^N,a(v)∣≤D2C(m+d+1)(m+1)C(m+1)(2d)m/2(1+∥v∥)−m. |\widehat F_{N,a}(v)| \le D_2^{C(m+d+1)}(m+1)^{C(m+1)} (2d)^{m/2}(1+\|v\|)^{-m}.

A shell T≤1+∥v∥<2TT\le1+\|v\|<2T contains at most (CT)2d(CT)^{2d} indices. Taking mm to be a sufficiently large fixed multiple of (d+1)2(d+1)^2 bounds the absolute coefficient sum over all groups in this shell by

D3T−2. D_3T^{-2}.

Since d≤log⁡Hd\le\log H, the prefactor for this fixed high derivative order is still quasipolynomial. The total absolute coefficient sum is therefore at most CD3CD_3, and the tail above T0T_0 is at most CD3T0−2CD_3T_0^{-2}. Given ε0>0\varepsilon_0>0, choose T0T_0 quasipolynomial in H,B,ε0−1H,B,\varepsilon_0^{-1}. This yields the uniform sup-norm truncation required in the main text.

The entries of the rational projection matrices have height at most BB. The number of such matrices is at most

(2B+1)2d2 (2B+1)^{2d^2}

We may first take the coefficient bounds above for every possible matrix and bounded group, then sum them. The cost is still quasipolynomial. Not every matrix needs to occur as a Weyl splitting at some scale. The actual splitting may vary within this fixed finite set.

Within the truncation range, all rational entries of N,P0,P1,Pf,Ps,p,ℓN,P_0,P_1,P_f,P_s,p,\ell have uniformly quasipolynomial height. Matrix multiplication, summation in fixed dimension, and clearing denominators also bound the height of σν\sigma_\nu quasipolynomially. For the rescaled family

V=rVy,Λ=r2Λy,b=rβy, V=rV_y,\quad\Lambda=r^2\Lambda_y,\quad b=r\beta_y,

the unscaled entries of the effective quadratic matrix are rational linear combinations of the entries of Λy\Lambda_y and pairwise products of entries of VyV_y. The linear frequencies are rational linear combinations of the entries of βy\beta_y and VyV_y.

We may therefore collect these finitely many unscaled real quantities into χy\chi_y. Its dimension is bounded by a fixed polynomial in the horizontal dimension, and all evaluation coefficients have height at most

exp⁡(C(1+log⁡H+log⁡B+log⁡(1/ε0))C). \exp\bigl(C(1+\log H+\log B+\log(1/\varepsilon_0))^C\bigr).

This is all the uniformity needed for the fixed-triple scale count. No numerical upper bound on large real frequencies is needed, and the same rational fast space need not work at every scale.

7. Scope of the verification

The derivation above reconstructs the Weyl output and finite expansion on pp. 16–20 used for the three-variable six-atom integral. The classical inputs are the explicitly stated upper bound in Minkowski's second theorem, together with Plancherel, integration by parts, and smooth periodic Fourier expansion in finite-dimensional Fourier analysis. The absolute convergence and quantitative tail of the last expansion have been developed in this appendix.

This appendix does not reconstruct the inverse theorem or detection lemma in Section 4, or supply the basic-catalog construction in Proposition 5.6. The main text develops the path budget and deletion error from the supplied basic data.