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Why three fixed basic columns leave only finitely many active scales

This chapter gives a close reading of Lemma 5.7 and Proposition 5.8 on pp. 37–38 of H. The fixed source is An L3L^3 bound for the trilinear Hilbert transform, October 5, 2026 version.

The catalog-termination argument in Chapter 9 needs two different counts: the number of original columns on a root-to-leaf path, and the number of active cells on that path. Having few original columns does not mean that the path is short. This chapter explains how oscillation of three fixed columns and the marginal cancellation of the kernel yield the second count, and states exactly where the first count comes from.

We start from the basic data already constructed on p. 37. Their construction and replacement errors in Proposition 5.6 on pp. 35–36 remain source inputs; this chapter does not infer that construction from the conclusions below. We develop the scale estimate for three fixed columns here. The three-variable analytic calculation is in the appendix to this chapter.

A companion proof of the source input above is now developed in H11: basic-column construction. Section 16 explains its original path-budget output. The proof retains the external discrete inverse theorem and explicit kernel conditions and does not use this chapter’s active-cell conclusion. The parameter note supplies a quantitative completion for the conventions on pp. 31 and 35. Actual later histories, whole helper bases, and global absorption are still not included.

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1. Original births, actual availability, and the whole-path budget

Fix a finite dyadic tree with root RR. Each basic label vv has a support-birth cell JvJ_v, a bounded basic scalar column ϕv\phi_v used on that cell, and a private coordinate:

Φv(y)=(ϕv(y),ϵv ev),y∈Jv. \Phi_v(y)=\bigl(\phi_v(y),\sqrt{\epsilon_v}\,e_v\bigr),\quad y\in J_v.

The scalar columns are quadratic chart atoms from Definition 4.1 on p. 15. Repeated occurrences of the same scalar function may still have different labels and different private coordinates. The slot is also part of the position at which an original column occurs.

Page 7 allows a projection to select only some of the columns already born. Let Vj(I)\mathcal V_j(I) be the basic list actually available in slot jj on cell II. The required conditions are

Vj(I)⊆{v:I⊆Jv},Vj(I)⊆Vj(I′) \mathcal V_j(I)\subseteq\{v:I\subseteq J_v\},\quad \mathcal V_j(I)\subseteq\mathcal V_j(I')

whenever I′I' is a child of II. Thus support birth and admission to a particular list may differ. Once admitted, a column is inherited by descendants. Refitting the coefficient of the same label on a descendant does not count as another birth. If an original label first becomes available farther down one branch, it must not be put into an ancestor's projection in advance.

For a complete root-to-leaf path π\pi, take the union of the basic labels that have been available on its cells, rather than summing the list sizes over cells. The original budget is

n0≥sup⁡π∑j=03#⋃I∈πVj(I).(original path budget) n_0\ge\sup_\pi\sum_{j=0}^3 \#\bigcup_{I\in\pi}\mathcal V_j(I). \tag{original path budget}

If we charge by support births, the condition on p. 7,

∑v1Jv(y)≤D \sum_v1_{J_v}(y)\le D

directly yields a stronger upper bound. Here finitely many basic catalogs may be combined, with occurrences in different slots counted separately.

On p. 37, DbaseD_{\mathrm{base}} is chosen to control these path counts, inverse private weights, atom complexity, and current coefficient sums simultaneously, and to satisfy

ek≤Dbase≤exp⁡(kC0).(basic budget) \mathrm e^k\le D_{\mathrm{base}}\le\exp(k^{C_0}). \tag{basic budget}

Page 39 also explicitly allows this basic budget to be enlarged to control the combined list of original vertices in all four slots. Denote the enlarged number by DD. We may therefore take an integer n0≤Dn_0\le D, with

log⁡n0≤log⁡D≤kC0. \log n_0\le\log D\le k^{C_0}.

This budget comes from the existing basic construction. It is not a new consequence of the active-cell count below.

2. Current basic parts and delayed differences

Fix two low slots i,ji,j, and denote the other two by a,ba,b. Page 37 writes

Yl=Bl+Ul,Ui=Uj=0, Y_l=B_l+U_l,\quad U_i=U_j=0,
Ue,I=(Pe,s+K0new−Pe,snew)Fe,e∈{a,b},s=depth⁡(I).(basic decomposition) U_{e,I}=(P^{\mathrm{new}}_{e,s+K_0}-P^{\mathrm{new}}_{e,s})F_e, \quad e\in\{a,b\},\quad s=\operatorname{depth}(I). \tag{basic decomposition}

The depth projections here are direct-sum projections over the corresponding refined partitions. Each BlB_l is the difference of at most two current basic projections. Its physical part on cell II therefore has a constant-coefficient representation

(Bl,I)phys=∑v∈Vl(I)cl,v,Iϕv,∑v∣cl,v,I∣≤D.(basic-column expansion) (B_{l,I})_{\mathrm{phys}} =\sum_{v\in\mathcal V_l(I)}c_{l,v,I}\phi_v, \quad \sum_v|c_{l,v,I}|\le D. \tag{basic-column expansion}

The coefficients may vary with II. We will not treat them as constants along a path.

The source inputs also include bounded local normalized norms for all current B,U,YB,U,Y in L2L^2, and normalization of the original inputs at the root:

∥Fe∥2,R≤CF,e∈{a,b}. \|F_e\|_{2,R}\le C_F,\quad e\in\{a,b\}.

The latter condition follows from the original LqL^q condition on the normalized tree on p. 4 and from q>2q>2. It cannot be inferred just from the sizes of B,U,YB,U,Y. This input normalization must also hold again when restricting to a new subroot. After increasing the starting parameter, DD can control these fixed constants as well. The later update layers also satisfy the following condition: any two full YY arguments have form norm at most the quantity below against arbitrary normalized L2(I)L^2(I) test functions in the other two slots:

η0=exp⁡(−kθ0),θ0>0.(full-argument pair-smallness) \eta_0=\exp(-k^{\theta_0}),\quad \theta_0>0. \tag{full-argument pair-smallness}

This condition comes from Proposition 5.6. It is not pair-smallness between pure basic columns, and does not say that every individual retained pattern is smaller than η0\eta_0.

3. The transpose norm of three fixed columns

Fix basic scalar columns in three different slots, and let ll be the empty slot. On cells where all three are available, set

AI=sup⁡∥f∥2,I≤1∣HI(ϕ0,…,f,…,ϕ3)∣,r=∣I∣, A_I=\sup_{\|f\|_{2,I}\le1} |H_I(\phi_0,\ldots,f,\ldots,\phi_3)|, \quad r=|I|,

where ll is the only slot containing ff. Each of the three fixed columns is bounded in absolute value by 11.

The normalized form on p. 4 of the source is

HI(z)=r−2∫R2wI(x,t)∏j=03zj(x+jt) dx dt. H_I(z)=r^{-2}\int_{\mathbb R^2} w_I(x,t)\prod_{j=0}^3z_j(x+jt)\,\mathrm dx\,\mathrm dt.

Set u=x+ltu=x+lt. The transpose function is then

TI(u)=r−1∫RwI(u−lt,t)∏j≠lϕj(u+(j−l)t) dt.(transpose function) T_I(u)=r^{-1}\int_{\mathbb R} w_I(u-lt,t)\prod_{j\ne l}\phi_j(u+(j-l)t)\,\mathrm dt. \tag{transpose function}

The kernel support implies that TIT_I is supported on II, and

HI(ϕ0,…,f,…,ϕ3)=1r∫If(u)TI(u) du,AI=∥TI∥2,I. H_I(\phi_0,\ldots,f,\ldots,\phi_3) =\frac1r\int_I f(u)T_I(u)\,\mathrm du, \quad A_I=\|T_I\|_{2,I}.

The last equality is L2L^2 duality for the bilinear pairing. If TI≠0T_I\ne0, we may take f=TI‾/∥TI∥2,If=\overline{T_I}/\|T_I\|_{2,I}.

The required estimate for three fixed columns has two parts. There are fixed C,pC,p such that, for 0<δ≤10<\delta\le1 and every spatial path,

#{I:AI>δ}≤C(1+log⁡D+log⁡(1/δ))p,(large-value scale count) \#\{I:A_I>\delta\} \le C\bigl(1+\log D+\log(1/\delta)\bigr)^p, \tag{large-value scale count}
∑I:AI≤δAI≤Cδ(1+log⁡D+log⁡(1/δ))p.(small-value path sum) \sum_{I:A_I\le\delta}A_I \le C\delta\bigl(1+\log D+\log(1/\delta)\bigr)^p. \tag{small-value path sum}

We sum only over cells where all three columns are already available. In fact, the proof controls the scales on their entire common-support subtree. Deleting unused cells cannot worsen these upper bounds.

4. Why we must fix a path point before rescaling

Choose a point yy on the path, so that every cell under consideration contains yy. In the square of the transpose norm, substitute

u=y+rh,t=rτ,t′=rτ′. u=y+rh,\quad t=r\tau,\quad t'=r\tau'.

The factors from the three differentials exactly cancel r−3r^{-3}, yielding

AI2=∫R3ΘI,y(h,τ,τ′)Qy(rh,rτ,rτ′) dh dτ dτ′,(six-atom integral) A_I^2=\int_{\mathbb R^3}\Theta_{I,y}(h,\tau,\tau') Q_y(rh,r\tau,r\tau')\,\mathrm dh\,\mathrm d\tau\,\mathrm d\tau', \tag{six-atom integral}

where

ΘI,y(h,τ,τ′)=wI(y+r(h−lτ),rτ)×wI(y+r(h−lτ′),rτ′)‾, \begin{aligned} \Theta_{I,y}(h,\tau,\tau') ={}&w_I\bigl(y+r(h-l\tau),r\tau\bigr)\\ &\times\overline{w_I\bigl(y+r(h-l\tau'),r\tau'\bigr)}, \end{aligned}
Qy(h,t,t′)=∏j≠lϕj(y+h+(j−l)t)ϕj(y+h+(j−l)t′)‾. Q_y(h,t,t')= \prod_{j\ne l}\phi_j\bigl(y+h+(j-l)t\bigr) \overline{\phi_j\bigl(y+h+(j-l)t'\bigr)}.

All the ΘI,y\Theta_{I,y} are supported in one fixed box and have uniform bounds for derivatives of each fixed order. They may vary independently from cell to cell.

After recentering every ϕj(y+z)\phi_j(y+z) at the same yy, set

aj=(1,j−l,0)T,bj=(1,0,j−l)T. a_j=(1,j-l,0)^T,\quad b_j=(1,0,j-l)^T.

The six atoms form one three-variable chart. Its unscaled horizontal matrix consists of the blocks

θjajT,θjbjT \theta_j a_j^T,\quad \theta_j b_j^T

and the corresponding diagonal blocks of the chart matrix are Cj,−CjC_j,-C_j. The ordinary quadratic matrix and linear vector are, respectively,

Λy=∑j≠lλj(ajajT−bjbjT),βy=∑j≠lβj,y(aj−bj). \Lambda_y=\sum_{j\ne l}\lambda_j(a_ja_j^T-b_jb_j^T), \quad \beta_y=\sum_{j\ne l}\beta_{j,y}(a_j-b_j).

The recentered parameters are now fixed. Their sizes may be arbitrarily large. The scale rr only changes these data to

Vr=rVy,Λr=r2Λy,br=rβy.(scaling fixed parameters) V_r=rV_y,\quad \Lambda_r=r^2\Lambda_y,\quad b_r=r\beta_y. \tag{scaling fixed parameters}

If we instead use each cell's own center without tracking the resulting changes in real parameters, there is no common parameter vector for the rational-height count below.

5. Why bounded rational height controls the number of scales

We first state the conclusion of Lemma 3.5 on pp. 13–14 that is actually used. Fix ξ∈Rd\xi\in\mathbb R^d, and consider all nonzero values produced by vectors whose entries have rational height at most B≥2B\ge2:

E={∣q⋅ξ∣:q∈Qd,ht⁡(q)≤B, q⋅ξ≠0}. \mathcal E=\{|q\cdot\xi|:q\in\mathbb Q^d, \operatorname{ht}(q)\le B,\ q\cdot\xi\ne0\}.

There is no bound on the size of ξ\xi.

If q1,…,qmq_1,\ldots,q_m is a minimally rationally dependent family, then m≤d+1m\le d+1. Clearing denominators column by column and then taking the maximal minors of a full-rank submatrix yields integers cic_i, all nonzero, such that

∑i=1mciqi=0,1≤∣ci∣≤Hd=d!Bd2+d.(short integer relation) \sum_{i=1}^m c_iq_i=0, \quad 1\le|c_i|\le H_d=d!B^{d^2+d}. \tag{short integer relation}

Minimal dependence ensures that the null vector obtained from these minors has no zero component.

Set Ld=4dHdL_d=4dH_d. If the absolute values of a sequence of nonzero evaluations are successively separated by factors greater than LdL_d, their rational vectors must be linearly independent. Otherwise, take a minimally dependent subfamily. In its integer relation, the term with the largest evaluation has absolute value at least that evaluation's absolute value, whereas the sum of the absolute values of all other terms is less than

dHd/Ld=1/4 dH_d/L_d=1/4

times the largest value. Cancellation is impossible.

Starting with the smallest value of E\mathcal E, cover it by [s,Lds][s,L_ds], then continue from the first uncovered value. Thus at most dd such intervals are needed. For rn=r02−nr_n=r_02^{-n} and ℓ∈{1,2}\ell\in\{1,2\}, the condition

α≤rnℓv≤β \alpha\le r_n^\ell v\le\beta

allows only one depth interval for each such interval, of length

ℓ−1(log⁡2Ld+log⁡2(β/α)) \ell^{-1}\bigl(\log_2L_d+\log_2(\beta/\alpha)\bigr)

Hence

#{n:∃v∈E,α≤rnℓv≤β}≤C(d+1)4(log⁡(2B)+log⁡(2β/α)).(rational-height scale bound) \#\{n:\exists v\in\mathcal E, \alpha\le r_n^\ell v\le\beta\} \le C(d+1)^4\bigl(\log(2B)+\log(2\beta/\alpha)\bigr). \tag{rational-height scale bound}

The sizes of the real parameters only move these intervals; they do not increase their number. Different rational coefficients may be chosen at each depth, because the set above includes all allowed coefficients from the outset.

6. A finite expansion of the three-variable chart at large-value scales

Write

K=1+log⁡D+log⁡(1/δ). K=1+\log D+\log(1/\delta).

If AI>δA_I>\delta, the six-atom integral has absolute value greater than δ2\delta^2 at Fourier frequency zero. The three-variable form of Lemma 4.3 on pp. 16–18 therefore yields a rational orthogonal splitting Pf+Ps=1P_f+P_s=1 whose height and slow horizontal part are bounded by

B1=exp⁡(CKC), B_1=\exp(CK^C),

and whose effective quadratic matrix satisfies

∥r2MPf∥≤B1, \|r^2M_{P_f}\|\le B_1,
MPf=Λy+12VyTCsyVy+sym⁡((PfVy)TCsk(PsVy)).(effective quadratic matrix) M_{P_f}=\Lambda_y+\frac12V_y^TC_{\mathrm{sy}}V_y +\operatorname{sym}\bigl((P_fV_y)^TC_{\mathrm{sk}}(P_sV_y)\bigr). \tag{effective quadratic matrix}

Here CC is the block matrix of the six atoms. Its symmetric and skew-symmetric parts, and sym⁡\operatorname{sym}, all use the division-by-two conventions in Section 2 of the appendix. The appendix derives each step from a large Fourier value to small return increments, a rational splitting, and then this matrix bound. It does not simply treat the previous chapter's one-parameter conclusion as a three-parameter conclusion.

Truncating the periodic Fourier expansion on pp. 18–20 on the fixed box to error ε0\varepsilon_0 yields

Qy(rz)=∑ν∈CIaI,νe(r2zTMPfz+rων⋅z)+EI(z),(finite chart expansion) Q_y(rz)= \sum_{\nu\in\mathcal C_I}a_{I,\nu} \mathrm e\bigl(r^2z^TM_{P_f}z+r\omega_\nu\cdot z\bigr) +E_I(z), \tag{finite chart expansion}
∥EI∥∞≤ε0,∑ν∣aI,ν∣≤B2,B2≤exp⁡(CKC) \|E_I\|_\infty\le\varepsilon_0, \quad \sum_\nu|a_{I,\nu}|\le B_2, \quad B_2\le\exp(CK^C)

when ε0\varepsilon_0 is a sufficiently small fixed multiple of δ2\delta^2. The coefficients and the splitting may change with the scale.

The important point is the form of the frequencies. They satisfy

ων=βy+VyTσν, \omega_\nu=\beta_y+V_y^T\sigma_\nu,

where the rational heights of σν\sigma_\nu have a uniform quasipolynomial upper bound. Put the entries of Λy\Lambda_y, βy\beta_y, and VyV_y, together with all pairwise products of entries of VyV_y, into one fixed real vector χy\chi_y. Then every entry of MPfM_{P_f} and every (ων)2(\omega_\nu)_2 has the form

q⋅χy,ht⁡(q)≤B3=exp⁡(CKC),dim⁡χy≤CKC.(fixed rational evaluation family) q\cdot\chi_y, \quad \operatorname{ht}(q)\le B_3=\exp(CK^C), \quad \dim\chi_y\le CK^C. \tag{fixed rational evaluation family}

All possible projection matrices, truncated frequencies, and periodic groups are included in this height bound. The coefficients may change, but they cannot produce a new family of unbounded rational height. The appendix derives the finite expansion and this uniformity explicitly.

7. Why the integral must be small at nonexceptional scales

After fixing the finite expansion and its absolute coefficient bound, choose

ε=δ2C∗B2,L=C∗B2δ2,(small and large thresholds) \varepsilon=\frac{\delta^2}{C_*B_2}, \quad L=\frac{C_*B_2}{\delta^2}, \tag{small and large thresholds}

where C∗C_* depends only on the fixed kernel class and fixed box, and is sufficiently large.

Declare the following two types of scales exceptional: some allowed nonzero quadratic entry satisfies

ε≤r2∣q⋅χy∣≤B1, \varepsilon\le r^2|q\cdot\chi_y|\le B_1,

or some allowed nonzero linear frequency in τ\tau satisfies

ε≤r∣q⋅χy∣≤L. \varepsilon\le r|q\cdot\chi_y|\le L.

The height bound in the preceding section and the scale bound in Section 5 imply that the total number of exceptional scales of both types is at most CKpCK^p. We first count over the entire allowed family of rational evaluations, then choose the actual splitting on each cell. Thus a scale-dependent splitting has not been treated as fixed.

Suppose a nonexceptional scale still has AI>δA_I>\delta. The Weyl splitting already bounds the effective quadratic entries by B1B_1, so all of them must be smaller than ε\varepsilon. Replacing the quadratic exponential by 11 on the fixed box costs at most CB2εCB_2\varepsilon.

In each remaining term, the τ\tau frequency has absolute value either below ε\varepsilon or above LL. For the large-frequency terms, integrate by parts once in τ\tau. The other linear factors are independent of τ\tau, so only the fixed kernel amplitude is differentiated. The total contribution is at most

CB2L−1. CB_2L^{-1}.

For the small-frequency terms, replace the τ\tau exponential by 11, at a total cost of at most CB2εCB_2\varepsilon. The resulting integral is exactly zero: for fixed h,τ′h,\tau', the other kernel and the remaining linear exponentials are independent of τ\tau, and

∫RwI(y+r(h−lτ),rτ) dτ=1r∫RwI(y+rh−lt,t) dt=0.(empty-slot marginal cancellation) \int_{\mathbb R} w_I\bigl(y+r(h-l\tau),r\tau\bigr)\,\mathrm d\tau =\frac1r\int_{\mathbb R}w_I(y+rh-lt,t)\,\mathrm dt=0. \tag{empty-slot marginal cancellation}

This is exactly the marginal condition in slot ll on p. 4.

Including the truncation error, the chosen constants ensure

AI2≤Cε0+CB2ε+CB2L−1≤12δ2, A_I^2\le C\varepsilon_0+CB_2\varepsilon+CB_2L^{-1} \le\frac12\delta^2,

contradicting AI>δA_I>\delta. Hence every large-value scale lies in the exceptional set, proving the large-value scale count. To respect the strict threshold range in Lemma 4.3, when δ≥1/2\delta\ge1/2 we may use the count at the fixed threshold 1/41/4. This changes only absolute constants.

8. From the large-value scale count to the small-value path sum

Partition 0<AI≤δ0<A_I\le\delta into the disjoint bands

2−m−1δ<AI≤2−mδ,m=0,1,2,…. 2^{-m-1}\delta<A_I\le2^{-m}\delta, \quad m=0,1,2,\ldots.

The number of terms in band mm is at most the large-value scale count at threshold 2−m−1δ2^{-m-1}\delta. Their sum is therefore at most

C2−mδ(K+(m+1)log⁡2)p. C2^{-m}\delta\bigl(K+(m+1)\log2\bigr)^p.

Since K≥1K\ge1,

∑m≥02−m(K+(m+1)log⁡2)p≤Kp∑m≥02−m(m+2)p≤CpKp. \sum_{m\ge0}2^{-m}\bigl(K+(m+1)\log2\bigr)^p \le K^p\sum_{m\ge0}2^{-m}(m+2)^p \le C_pK^p.

Zero terms contribute nothing. This proves the small-value path sum, including terms equal to the threshold.

Knowing only that AI≤δA_I\le\delta on every inactive cell is not enough. Even with AIm=δ/(m+1)A_{I_m}=\delta/(m+1), every term is small but the path sum can still grow with depth. This section uses the same polynomial count at every smaller threshold.

9. Active cells and the root-to-leaf path count

Now fix a sufficiently large absolute constant AA and set

δ=D−A. \delta=D^{-A}.

A cell II is active if and only if there are actually available pure basic columns in three different slots whose transpose norm is greater than δ\delta. This definition applies to all retained patterns at once, regardless of whether a pattern's current coefficient is zero.

On a complete path, take the union of all basic labels, counting them by slot. Their total number is at most DD. Thus there are at most D3D^3 triples from different slots. Each fixed triple is tested only after all three columns are available, and its number of active scales is at most

C(1+(A+1)log⁡D)p. C\bigl(1+(A+1)\log D\bigr)^p.

Taking the union over all triples yields

M≤CD3(1+(A+1)log⁡D)p≤D4(active path budget) M\le CD^3\bigl(1+(A+1)\log D\bigr)^p\le D^4 \tag{active path budget}

for a sufficiently large starting kk. The last explicit exponent is not asserted to be optimal in the source. It is a convenient bound once the fixed parameters have been chosen; the source only needs M≤DCM\le D^C.

If the tree has many disjoint branches, its total number of original labels may be large. The count is always taken on one path. Triples from other branches are not added to the current path.

10. Summing the error from deleting inactive cells by length

Each retained pattern has at least three BB arguments. Fix three of their slots and expand their basic columns, leaving the fourth whole argument unchanged. The basic-column expansion and the definition of the transpose norm imply, on an inactive cell,

∣HI(z)∣≤∥zl,I∥2,I∑v1,v2,v3∣c1,v1,Ic2,v2,Ic3,v3,I∣AI;v1,v2,v3. |H_I(z)|\le \|z_{l,I}\|_{2,I} \sum_{v_1,v_2,v_3} |c_{1,v_1,I}c_{2,v_2,I}c_{3,v_3,I}|A_{I;v_1,v_2,v_3}.

To avoid extra assumptions on the changing coefficients, we may use the following bounds term by term:

∥zl,I∥2,I≤D,∣c1,v1,Ic2,v2,Ic3,v3,I∣≤D3. \|z_{l,I}\|_{2,I}\le D, \quad |c_{1,v_1,I}c_{2,v_2,I}c_{3,v_3,I}|\le D^3.

On a fixed path, first sum by triples. Every triple that occurs satisfies AI;v1,v2,v3≤δA_{I;v_1,v_2,v_3}\le\delta on these inactive cells, so Section 8 yields

∑I∈π inactive∣HI(z)∣≤CD4D3δ(1+(A+1)log⁡D)p≤CD7−A(1+(A+1)log⁡D)p.(inactive path error) \begin{aligned} \sum_{I\in\pi\,\mathrm{inactive}}|H_I(z)| &\le CD^4D^3\delta \bigl(1+(A+1)\log D\bigr)^p\\ &\le CD^{7-A}\bigl(1+(A+1)\log D\bigr)^p. \end{aligned} \tag{inactive path error}

We spend an extra fixed power rather than incorrectly pulling the cell-dependent coefficients outside the whole path sum for a fixed triple.

This decomposition has three retained patterns in total. We may take A=10A=10. After fixing p,Cp,C, increase the starting kk so that the total path error of all three patterns is at most D−1D^{-1}. Finally, use the finite-sum Fubini identity

∑I inactive∣I∣ ∣HI(z)∣=∫R∑I∋y inactive∣HI(z)∣ dy.(paths to length sums) \sum_{I\,\mathrm{inactive}}|I|\,|H_I(z)| =\int_R\sum_{I\ni y\,\mathrm{inactive}}|H_I(z)|\,\mathrm dy. \tag{paths to length sums}

Summing all retained patterns, the error is at most

D−1∣R∣≤e−k∣R∣. D^{-1}|R|\le\mathrm e^{-k}|R|.

If the local sizes or basic coefficient sums were initially bounded by other fixed powers of DD, simply increase AA after fixing these costs. The remaining parameter order is unchanged.

11. Why the two delayed differences can be estimated first

For a high slot, write on the whole refined tree

Δh=Ph+1new−Phnew. \Delta_h=P^{\mathrm{new}}_{h+1}-P^{\mathrm{new}}_h.

Inheritance ensures that these are mutually orthogonal projection increments, and

Ue,I=1I∑j=0K0−1Δs+jFe. U_{e,I}=1_I\sum_{j=0}^{K_0-1}\Delta_{s+j}F_e.

For fixed jj, first sum over disjoint cells at the same depth, then use the orthogonality of all Δh\Delta_h. The total squared norm of the corresponding row vector is at most ∥1RFe∥22\|1_RF_e\|_2^2. Applying the triangle inequality over jj in the row Hilbert space yields

∑I⊆R∣I∣∥Ue,I∥2,I2≤K02∥1RFe∥22≤C(1+K0)2∣R∣.(delayed-difference square sum) \sum_{I\subseteq R}|I|\|U_{e,I}\|_{2,I}^2 \le K_0^2\|1_RF_e\|_2^2 \le C(1+K_0)^2|R|. \tag{delayed-difference square sum}

If K0=0K_0=0, the left side is zero. If the tree ends too soon, continue inheriting the existing columns and refitting locally, as prescribed on p. 7, to supply the required finite refinement. No new columns are needed.

The two low slots have no UU, so the only pattern containing two UU arguments is

HI(Yi,Yj,Ua,Ub). H_I(Y_i,Y_j,U_a,U_b).

Full-argument pair-smallness and Cauchy–Schwarz yield

∑I∣I∣ ∣HI(Yi,Yj,Ua,Ub)∣≤Cη0(1+K0)2∣R∣. \sum_I|I|\,|H_I(Y_i,Y_j,U_a,U_b)| \le C\eta_0(1+K_0)^2|R|.

For the finitely many initial update layers where η0\eta_0 is unavailable, the same local absolute L2L^2 estimate still yields a bound independent of tree depth.

12. Why a minimum appears at the end

For the later update layers, the source input implies

∣HI(Y)∣≤C1η0. |H_I(Y)|\le C_1\eta_0.

Choose a smaller but still positive fixed exponent θ<θ0\theta<\theta_0 and increase the starting kk, so that

C1η0≤η=exp⁡(−kθ). C_1\eta_0\le\eta=\exp(-k^\theta).

Expand the full YY into the three retained patterns and the two-difference pattern above. Apply the triangle inequality first, then use

min⁡(η,∑jxj)≤∑jmin⁡(η,xj),xj≥0. \min\left(\eta,\sum_jx_j\right) \le\sum_j\min(\eta,x_j),\quad x_j\ge0.

Thus

∣HI(Y)∣≤∑z retainedmin⁡(η,∣HI(z)∣)+∣HI(Yi,Yj,Ua,Ub)∣.(minimum reduction) |H_I(Y)|\le \sum_{z\,\mathrm{retained}}\min\bigl(\eta,|H_I(z)|\bigr) +|H_I(Y_i,Y_j,U_a,U_b)|. \tag{minimum reduction}

On inactive cells, use min⁡(η,x)≤x\min(\eta,x)\le x and the absolute error from Section 10. What remains is exactly equation (11)(11) of Proposition 5.8: estimate each sum

∑I active∣I∣min⁡(η,∣HI(z)∣). \sum_{I\,\mathrm{active}}|I|\min\bigl(\eta,|H_I(z)|\bigr).

We do not claim that every HI(z)H_I(z) has the pair-smallness of the full YY. For the finitely many initial layers, it suffices to use the active path budget, the local absolute estimate, and the path-to-length identity. The constants may depend on those fixed layers, but not on the total depth.

13. What is preserved on restriction to a subroot

The active cells need not form an ancestor-closed tree. When a tree is needed, add the root and the cells connecting the active cells to it. The budget MM counts only active cells; there may still be many connecting cells. The original budget n0n_0 must cover all original births on each complete path, including columns born on connecting cells and first used at deeper active cells.

When restricting to a subroot R′R' that already satisfies the required local normalization, keep the original functions, private labels, and lists. Labels already available above the subroot are inherited at the new root and are not charged again. Births below the subroot must not be used in the new root's projection in advance. Each new path extends to an original path, so the upper bounds for n0n_0 and MM remain valid. The orthogonal square-sum estimate in Section 11 can be proved again on R′R'.

When later removing filters from the two nonside slots, one must return to this tuple's original whole BB arguments. For these two slots p,qp,q, the identity

BpBq=YpYq−UpYq−YpUq+UpUq B_pB_q=Y_pY_q-U_pY_q-Y_pU_q+U_pU_q

shows that restoring the full Yp,YqY_p,Y_q allows the main term to use the source-input pair-smallness, while every other term contains an additional basic side argument. The whole BB cannot be replaced here by a selected subset of basic columns. That would not recover the original YY through the same identity.

These are inheritance conventions for the spatial tree and basic data. The actual center witnesses in the historical ball masks on p. 43, and the projection words required for testing on pp. 47–49, are separately defined later. The active path budget itself neither lists those projection histories nor verifies their number.

14. Parameter order and the scope left open by this chapter

First fix the basic catalog, K0K_0, local sizes, and full-argument pair-smallness supplied by Proposition 5.6. Then choose DD to control these basic data. The exponent in the fixed-triple estimate depends only on the atom-complexity rules and fixed kernel class, not on real frequencies, tree depth, the number of branches, or the birth locations of the triple.

Next fix the active-threshold exponent AA. Only then, for each required threshold δ\delta, choose the Weyl-splitting budget, Fourier truncation, and small/large frequency gap. The actual splitting and truncation may vary by cell, but their rational heights must lie in a uniformly fixed range. Finally increase the starting kk to absorb fixed polynomial factors and set MM and the original budget n0n_0 used in Chapter 9. New template insertions in Chapter 9 do not redefine activity in this chapter or add to its original vertices.

Under these explicit basic-data assumptions, this chapter proves the fixed-triple large-value scale count, small-value path sum, active path budget, and minimum reduction after removing inactive cells and the two-difference term. The appendix derives the three-variable Weyl estimate and finite chart expansion.

The parts not reconstructed here are the actual construction in Proposition 5.6 and of earlier original catalogs, the spatial compression in the full Lemma 3.4, the actual localization errors and history lists in Proposition 6.8, the whole helper bases in Section 7, and the global absorption argument for H. In particular, the numerical budget for n0n_0 still comes from the basic construction on p. 37. This chapter only aligns that source with the counting objects actually needed later. It does not establish closure of the whole paper H.