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.

Unit 3, continued: counting core tuples and interpolating amplitudes

This part develops D §6.6, pp.57–58, equations (6.23)–(6.24). The corresponding source argument is H §9 in the October 5, 2026 version, especially Proposition 9.2 (pp.87–88) and Proposition 9.3 (pp.89–90).

The preceding part treated two side-function positions. Here at least three positions are core. One interval may contain many representative tuples; taking a power below one separately for every tuple would lose the counting gain. We therefore retain each group's full count and sum successively over depths, groups, amplitudes, and frequencies.

The scalar kernel calculations in H §§9.1–9.2 remain inputs. The finite combinatorial proof of Lemma 9.1 is given in Finite counting on sparse scales. We state the conclusions and hypotheses used here, check what changes with D's varying functions, derive power-count bounds from sparse mass, and carry out the interpolation and summation.

1. Fixed data and the quantity being counted

Fix a point x∗x_* on a retained path, a group GG, an upper height, the types in each position, frequency parameters (μ,ν,Λ)(\mu,\nu,\Lambda), and four amplitude classes σj\sigma_j. Here

0<μ≤1≤ν,Λ≥1 0<\mu\le1\le\nu,\qquad \Lambda\ge1

take dyadic values. If all four positions are core, set Λ=1\Lambda=1.

At depth ss, write the path interval as IsI_s, its length as rsr_s, and its reciprocal scale as Rs=rs−1R_s=r_s^{-1}. The real number assigned to representative label aa is

γa=ωa(x∗). \gamma_a=\omega_a(x_*).

The same label uses this value at every depth.

Let NsGN_s^G count the tuples of core representative labels passing the source frequency test for these fixed data. A tuple is counted at most once at each depth. These are the tuples retained by the actual scalar calculation, not an arbitrary set of tuples with roughly nearby frequencies.

For core position jj, denote the label set by AjG\mathcal A_j^G and define

MjG=∣AjG∣. M_j^G=|\mathcal A_j^G|.

If there is a side position ll, define

MlG=σl−2∑s: G used on Is ∥Sl,G,s∥2,Is 2,M′=max⁡0≤j≤3MjG.(Role-count) M_l^G=\sigma_l^{-2} \sum_{s:\,G\text{ used on }I_s\text{ }} \|S_{l,G,s}\|_{2,I_s}^{\,2}, \qquad M'=\max_{0\le j\le3}M_j^G. \tag{Role-count}

The normalized local norm is

∥f∥2,I 2=∣I∣−1∫I∣f∣2. \|f\|_{2,I}^{\,2}=|I|^{-1}\int_I|f|^2.

Omit groups with no nonzero count. Every remaining group satisfies M′≥1M'\ge1. For a nonzero use in the side position, the Fourier-window size below is at least σl\sigma_l, and Parseval gives the same conclusion.

2. The scalar quantities and their sources

2.1 Common heights, complete components, and errors

For a core tuple, H §9.1 samples common heights and takes the first at which every core position succeeds. Failures are assigned only to positions. Both success and failure conditions select complete core partial sums within minimal CURRENT components, which may also contain side modes. A core partial sum is not cut anew according to the size of one Fourier mode inside its component.

Let the number of core positions be m0∈{3,4}m_0\in\{3,4\}. Among the preceding nn failures, let njn_j be assigned to position jj. The source core size σFj\sigma_{F_j} and torus-function size aj′a_j' satisfy

aj′≤CσFj,E(aj′)2≤C(2δ∗)njσFj2. a_j'\le C\sigma_{F_j}, \qquad \mathbb E(a_j')^2 \le C(2\delta_*)^{n_j}\sigma_{F_j}^2.

Use the deterministic bound to raise the second moment to the m0m_0-th moment, then apply Hölder:

E∏jaj′≤Cm0(2δ∗)n/m0∏jσFj. \mathbb E\prod_j a_j' \le C^{m_0}(2\delta_*)^{n/m_0}\prod_j\sigma_{F_j}.

At length nn, there are at most m0nm_0^n failure-position records. Thus, for a sufficiently small fixed δ∗\delta_*,

∑n≥0m0n(2δ∗)n/m0<∞. \sum_{n\ge0}m_0^n(2\delta_*)^{n/m_0}<\infty.

The failure records therefore introduce no additional factor growing with depth.

Scalar approximation, Fourier tails, and discarded small terms are bounded absolutely before taking powers, with total O(e−k∣R∣)O(e^{-k}|R|). This error is not subsequently raised to the pp-th power and resummed.

2.2 The frequency tests

Retain H's horizontal frequency vector and height scales, and write

ξ=ϑfreq/Lh−Δ,U0=D∗250. \xi=\vartheta_{\rm freq}/L_{h-\Delta}, \qquad U_0=D_*^{250}.

The frequency vector ϑfreq\vartheta_{\rm freq} is distinct from the small scalar interpolation parameter ϑ\vartheta used later. The retained frequency range is

U0−1≤μ≤1≤ν,Λ≤CU0. U_0^{-1}\le\mu\le1\le\nu,\Lambda\le C U_0.

At the end we may enlarge these finite ranges when summing.

For four core positions, set

Q=∑j=03γj,T=∑j=03jγj. Q=\sum_{j=0}^3\gamma_j,\qquad T=\sum_{j=0}^3j\gamma_j.

Choose reference vectors n,mn,m in the complete finite shift range so that

q′=Q+n⋅ξ,t′=T+m⋅ξ q'=Q+n\cdot\xi,\qquad t'=T+m\cdot\xi

lie in the permitted intermediate-frequency range. Use a fixed rule for these references, independent of later failure records or component selections. The parameters satisfy

μ≍min⁡(1,min⁡0≤j≤3∣t′−jq′∣Rs),ν≍max⁡(1,∣q′∣Rs,∣t′∣Rs).(Four-test) \mu\asymp \min\left(1,\min_{0\le j\le3}\frac{|t'-jq'|}{R_s}\right), \qquad \nu\asymp\max\left(1,\frac{|q'|}{R_s},\frac{|t'|}{R_s}\right). \tag{Four-test}

For three core positions and side position ll, set

Q=∑j≠lγj,Tl=∑j≠l(j−l)γj. Q=\sum_{j\ne l}\gamma_j,\qquad T_l=\sum_{j\ne l}(j-l)\gamma_j.

Choose a permitted mm and classify by

β=rs(Tl+m⋅ξ),μ≍min⁡(1,∣β∣),ν≍max⁡(1,∣β∣)(Three-test) \beta=r_s(T_l+m\cdot\xi),\qquad \mu\asymp\min(1,|\beta|),\qquad \nu\asymp\max(1,|\beta|) \tag{Three-test}

Very small nonzero parameters and cases without an intermediate-frequency reference have already been included in the absolute error.

Use the actual side function Sl,G,sS_{l,G,s} on the current interval. Insert a newly sampled translated cutoff and remove its fixed quadratic phase to obtain S′S', with

∥S′∥2,Is≤∥Sl,G,s∥2,Is. \|S'\|_{2,I_s}\le\|S_{l,G,s}\|_{2,I_s}.

The corresponding window size is

bΛ2=Eρl∑k′∈Z:∣k′+rs(Q+n⋅ξ)∣≤2Λfor some permitted n∣S′^Is(k′)∣2.(Side-window) b_\Lambda^2= \mathbb E_{\rho_l} \sum_{\substack{k'\in\mathbb Z:\\ |k'+r_s(Q+n\cdot\xi)|\le2\Lambda\\ \text{for some permitted }n}} |\widehat{S'}_{I_s}(k')|^2. \tag{Side-window}

The shift vector nn ranges over the full Fourier range, so the window does not change with the failure record. Different tuples on the same cell are tested using the same new shift ρl\rho_l. The side amplitude σl\sigma_l is the dyadic class containing bΛb_\Lambda.

2.3 The scalar input used here

H §9.2 states that, after removing the absolute errors above, the interval contribution for fixed data is bounded by

CLμν−LΛ−L(∏j=03σj)NsG(Cell-core) C_L\mu\nu^{-L}\Lambda^{-L} \left(\prod_{j=0}^3\sigma_j\right)N_s^G \tag{Cell-core}

where LL is any sufficiently large fixed integer.

The factor μ\mu comes from the kernel's vanishing marginals; ν−L\nu^{-L} comes from its smooth far-frequency decay. With three core positions, Λ−L\Lambda^{-L} comes from decay in pairing the side-function Fourier windows. Four core positions use a four-factor L2L^2 estimate on the torus; three core positions use its dual form and Parseval. These require the full frequency-shift range, pure-shift gap, and height margins retained in H's construction. Equation (Cell-core) is a specified input here, not a consequence of representative separation alone.

3. The complete finite sparse-counting statement

H Lemma 9.1 (pp.81–87) uses the following finite data.

There are four positions 0,1,2,30,1,2,3, three or four of which are core, forming the set J\mathcal J. Given

M,L≥1,d≥0,B≥1,0<μ≤1≤ν, M,L\ge1,\quad d\ge0,\quad B\ge1,\quad 0<\mu\le1\le\nu,

each core position has a finite real-label set Ai\mathcal A_i with ∣Ai∣≤M|\mathcal A_i|\le M. Within a position, the assignment of labels to real numbers is injective. Also fix ζ∈Rd\zeta\in\mathbb R^d.

At finitely many distinct integers ss, take

Rs=R0 2s,Es⊆∏i∈JAi,Ns=∣Es∣. R_s=R_0\,2^s,\qquad E_s\subseteq\prod_{i\in\mathcal J}\mathcal A_i,\qquad N_s=|E_s|.

Assume:

(1) Labels in two distinct core positions determine at most one complete core tuple, and that pair of labels appears at at most LL scales. (2) If there is a side position ll, there are weights ws≥0w_s\ge0 with ∑sws≤M\sum_s w_s\le M such that at depth ss at most wsw_s tuples contain any specified core label. (3) If distinct labels a,a′a,a' in one core position appear at scales s,ts,t, then for every integer vector satisfying ∣n∣∞≤Q|n|_\infty\le Q,

∣a−a′+n⋅ζ∣>Σmax⁡(Rs,Rt).(Separation) |a-a'+n\cdot\zeta|>\Sigma\max(R_s,R_t). \tag{Separation}

(4) For every three-core subset T⊆J\mathcal T\subseteq\mathcal J, let l′l' be the omitted position. Every tuple at scale ss has an integer vector satisfying ∣n∣∞≤B|n|_\infty\le B such that

μRs≤∣∑i∈T(i−l′)ai+36n⋅ζ∣≤νRs.(Annulus) \mu R_s\le \left|\sum_{i\in\mathcal T}(i-l')a_i+36n\cdot\zeta\right| \le\nu R_s. \tag{Annulus}

(5) At every scale ss with a tuple, for all ∣n∣∞≤Q|n|_\infty\le Q,

∣n⋅ζ∣∉[μRs/1000, 1000νRs].(Pure-gap) |n\cdot\zeta|\notin [\mu R_s/1000,\,1000\nu R_s]. \tag{Pure-gap}

Also require

Q≥Cres(d+1)2B,Σ≥Cres(d+1)2ν. Q\ge C_{\rm res}(d+1)^2B,\qquad \Sigma\ge C_{\rm res}(d+1)^2\nu.

Then for 0<δ≤10<\delta\le1,

∑s: Ns≤δM2Ns≤CℓL29δ1/2080M2,ℓ=1+log⁡2 ⁣(2+(d+1)2ν/μ).(Sparse-mass) \sum_{s:\,N_s\le\delta M^2}N_s \le C\ell L^{29}\delta^{1/2080}M^2, \quad \ell=1+\log_2\!\left(2+(d+1)^2\nu/\mu\right). \tag{Sparse-mass}

The constant is independent of the number of scales, the number of labels, and the particular real frequencies.

We use this conclusion below; its four-step-path and slab-covering proof is developed in the linked extension. The annulus and pure-gap assumptions are substantive and cannot be replaced by uniqueness from two labels.

4. Conditions to recheck for D's varying functions

4.1 Two core labels determine the remaining labels

With four core positions, suppose two tuples share labels in positions i,ji,j, leaving positions a,ba,b. Subtract their Q,TQ,T tests. The unknown differences satisfy an approximate two-variable linear system with matrix

(11ab). \begin{pmatrix}1&1\\a&b\end{pmatrix}.

Its determinant is b−ab-a, with absolute value in {1,2,3}\{1,2,3\}. The unknown differences therefore lie in ranges described by finite shifts and an error O(νmax⁡(Rs,Rt))O(\nu\max(R_s,R_t)). The separation margin allows these subtractions, integer divisions, and shifts, forcing equal labels in both remaining positions.

With three core positions and two labels fixed, one equation for TlT_l determines the remaining label. Its coefficient is the nonzero integer j−lj-l of absolute value at most three, and the same separation margin gives uniqueness.

The separation scale is max⁡(Rs,Rt)\max(R_s,R_t), so this also compares different depths. The number of scales at which a complete tuple passes the test is controlled by H's height-grouping result:

L0≤PC(1+log⁡(ν/μ))C.(Scale-count) L_0\le P^C(1+\log(\nu/\mu))^C. \tag{Scale-count}

This step uses the frequency-annulus test as well as label uniqueness.

4.2 Incidence counts between core and side positions

Fix one core label and one scale. If two distinct three-core tuples have overlapping windows in (Side-window), their QQ frequencies differ, after finite shifts, by O(ΛRs)O(\Lambda R_s). Combining this with their two TlT_l equations again gives a two-variable system with determinant of absolute value at most three. Source separation is much larger than the allowed ν,Λ\nu,\Lambda, so the other two labels must agree.

The windows of distinct tuples are therefore disjoint. Every counted tuple satisfies bΛ≥σlb_\Lambda\ge\sigma_l. Apply Parseval for the same newly sampled shift, then take expectation, to obtain

#{tuples containing this core label}≤σl−2∥Sl,G,s∥2,Is 2=:ws.(Incidence) \#\{\text{tuples containing this core label}\} \le \sigma_l^{-2}\|S_{l,G,s}\|_{2,I_s}^{\,2} =:w_s. \tag{Incidence}

Summing over scales gives exactly ∑sws=MlG\sum_s w_s=M_l^G.

This calculation requires the actual side function on the current cell. Older frozen coefficients from different blocks may be unrelated and cannot be treated as one common Fourier sequence.

4.3 Inherited frequency gaps

To apply the finite lemma, H sets

ζ=ξ/36,M=M′,L=L0. \zeta=\xi/36,\qquad M=M',\qquad L=L_0.

Equations (Four-test) and (Three-test) supply the annulus test for every three-core subset. To check the finite lemma's two numerical requirements, the source uses

ζ=ξ36=6Δ−2ϑfreqLh,Bh′=D∗5Eh−Δ, \zeta=\frac{\xi}{36} =6^{\Delta-2}\frac{\vartheta_{\rm freq}}{L_h}, \qquad B_h'=D_*^5E_{h-\Delta},
Qres=⌊Eh/6Δ−2⌋,Σ=Ξ/2,Ξ=D∗1000,B=CBh′.(Count-reserves) Q_{\rm res}= \left\lfloor E_h/6^{\Delta-2}\right\rfloor, \qquad \Sigma=\Xi/2,\qquad \Xi=D_*^{1000}, \qquad B=C B_h'. \tag{Count-reserves}

Here QresQ_{\rm res} is the parameter QQ in the finite lemma. The quantities Eh,LhE_h,L_h are the shift range and denominator scale in the original height construction. The equality uses Lh/Lh−Δ=6ΔL_h/L_{h-\Delta}=6^\Delta. H's choice of the height parameter A0A_0 gives

Qres≥Cres(d+1)2B. Q_{\rm res}\ge C_{\rm res}(d+1)^2B.

Moreover, ν≤CD∗250\nu\le C D_*^{250}, the horizontal dimension satisfies the previously fixed bound, and Ξ=D∗1000\Xi=D_*^{1000}. The source separation parameter therefore ensures

Σ≥Cres(d+1)2ν. \Sigma\ge C_{\rm res}(d+1)^2\nu.

Fixed constants in the annulus bounds are absorbed by decreasing μ\mu and increasing ν\nu by fixed factors. The margins above remain valid.

The pure-shift gap uses at least one nonexceptional main label in every successful component. The representative itself may be exceptional; a suitable main label in the same component is what is needed. The source rational-height bound HH covers all pure horizontal shifts in (Count-reserves). For them, the source frequency dichotomy gives

∣n⋅ζ∣≤T−1/rvbor∣n⋅ζ∣≥T/rtb. |n\cdot\zeta|\le T^{-1}/r_{v_b} \quad\text{or}\quad |n\cdot\zeta|\ge T/r_{t_b}.

The reciprocal scale of a tested cell lies between rvb−1r_{v_b}^{-1} and rtb−1r_{t_b}^{-1}. Together with μ≥U0−1\mu\ge U_0^{-1} and ν≤CU0\nu\le CU_0, the source choice of TT makes the first alternative strictly less than μRs/1000\mu R_s/1000 and the second strictly greater than 1000νRs1000\nu R_s. This verifies (Pure-gap).

These numerical relations are hypotheses inherited from H's construction. We check their correspondence to the finite lemma's conditions without reproving the entire mode-graph and height construction.

The parts affected by D's new functions are thus the fixed representative values, positionwise counts, and actual side-function square sizes. The other frequency tests and gaps remain those of H.

5. Two counting bounds

For any distinct positions i,ji,j, the incidence counts above give

∑sNsG≤L0MiGMjG.(Count-one) \sum_sN_s^G\le L_0M_i^GM_j^G. \tag{Count-one}

For two core positions, this counts label pairs times their scale multiplicity. For one core and one side position, it follows from (Incidence), and remains true after multiplication by L0≥1L_0\ge1.

The finite sparse-mass lemma gives an absolute c′>0c'>0, for example c′=1/2080c'=1/2080, such that

∑s: NsG≤δ(M′)2NsG≤PC(1+ν+μ−1+Λ)Cδc′(M′)2.(Small-count-mass) \sum_{s:\,N_s^G\le\delta(M')^2}N_s^G \le P^C(1+\nu+\mu^{-1}+\Lambda)^C \delta^{c'}(M')^2. \tag{Small-count-mass}

The coefficient includes the dimension, logarithms, and L0L_0 cost from (Sparse-mass).

Uniqueness from two core labels gives

NsG≤(M′)2. N_s^G\le(M')^2.

Choose

p0=1−c′2∈(0,1). p_0=1-\frac{c'}2\in(0,1).

On scales satisfying

2−h−1(M′)2<NsG≤2−h(M′)2 2^{-h-1}(M')^2<N_s^G\le2^{-h}(M')^2

the inequality p0−1<0p_0-1<0 gives

(NsG)p0=NsG(NsG)−(1−p0)≤NsG(2h+1(M′)2)1−p0. (N_s^G)^{p_0} =N_s^G(N_s^G)^{-(1-p_0)} \le N_s^G \left(\frac{2^{h+1}}{(M')^2}\right)^{1-p_0}.

Apply (Small-count-mass) and sum over h≥0h\ge0 to obtain

∑s(NsG)p0≤CPC(1+ν+μ−1+Λ)C(M′)2p0∑h≥02h(1−p0−c′)≤PC(1+ν+μ−1+Λ)C(M′)2p0.(Count-small-power) \begin{aligned} \sum_s(N_s^G)^{p_0} &\le C P^C(1+\nu+\mu^{-1}+\Lambda)^C (M')^{2p_0} \sum_{h\ge0}2^{h(1-p_0-c')}\\ &\le P^C(1+\nu+\mu^{-1}+\Lambda)^C(M')^{2p_0}. \end{aligned} \tag{Count-small-power}

Here 1−p0−c′=−c′/2<01-p_0-c'=-c'/2<0. This is the second estimate in D (6.23). Zero-count scales contribute nothing.

6. Interpolating the two counts

Choose a small absolute number ϑ∈(0,1)\vartheta\in(0,1), to be fixed later, and define

p=(1−ϑ)+ϑp0=1−ε,ε=ϑ(1−p0)>0. p=(1-\vartheta)+\vartheta p_0 =1-\varepsilon,\qquad \varepsilon=\vartheta(1-p_0)>0.

Hölder gives directly

∑s(NsG)p=∑s(NsG)1−ϑ((NsG)p0)ϑ≤(∑sNsG)1−ϑ(∑s(NsG)p0)ϑ≤(L0MiGMjG)1−ϑ[PC(1+ν+μ−1+Λ)C(M′)2p0]ϑ.(Interpolated-count) \begin{aligned} \sum_s(N_s^G)^p &=\sum_s (N_s^G)^{1-\vartheta} \big((N_s^G)^{p_0}\big)^\vartheta\\ &\le \left(\sum_sN_s^G\right)^{1-\vartheta} \left(\sum_s(N_s^G)^{p_0}\right)^\vartheta\\ &\le (L_0M_i^GM_j^G)^{1-\vartheta} \left[ P^C(1+\nu+\mu^{-1}+\Lambda)^C(M')^{2p_0} \right]^\vartheta. \end{aligned} \tag{Interpolated-count}

The count NsGN_s^G remains intact inside its power; it has not been expanded into NsGN_s^G unit terms.

7. Summing over groups using total degree greater than one

The preceding component-size and top counts, together with the side-function pathwise square sums, give for each position

∑GMiG≤CPCσi−2.(Role-total) \sum_GM_i^G\le C P^C\sigma_i^{-2}. \tag{Role-total}

A core position also satisfies

∑GMiG≤D∗.(Core-cap) \sum_GM_i^G\le D_*. \tag{Core-cap}

The source logarithmic growth condition absorbs later factors of log⁡D∗\log D_* into permitted polynomials in P,kP,k. It does not treat D∗D_* itself as a small power of PP.

We need the elementary fact that, if miG≥0m_i^G\ge0, βi≥0\beta_i\ge0, and

B=∑iβi≥1, B=\sum_i\beta_i\ge1,

then

∑G∏i(miG)βi≤∏i(∑GmiG)βi.(Group-sum) \sum_G\prod_i(m_i^G)^{\beta_i} \le\prod_i\left(\sum_Gm_i^G\right)^{\beta_i}. \tag{Group-sum}

To prove it, omit zero-exponent positions. If a required sum vanishes, both sides vanish. Otherwise normalize by

aiG=miG/∑GmiG,∑GaiG=1. a_i^G=m_i^G\Big/\sum_Gm_i^G, \qquad \sum_Ga_i^G=1.

Hölder with exponents B/βiB/\beta_i gives

∑G∏i(aiG)βi≤∏i(∑G(aiG)B)βi/B≤1, \sum_G\prod_i(a_i^G)^{\beta_i} \le \prod_i\left(\sum_G(a_i^G)^B\right)^{\beta_i/B} \le1,

using 0≤aiG≤10\le a_i^G\le1 and B≥1B\ge1 in the last step.

In (Interpolated-count), split M′=max⁡iMiGM'=\max_iM_i^G into at most four cases according to where the maximum occurs. Each term has total degree

2(1−ϑ)+2ϑp0=2p. 2(1-\vartheta)+2\vartheta p_0=2p.

We will choose p>2/3p>2/3, so 2p>12p>1 and (Group-sum) applies.

8. Three amplitude ratios and one common scale

Temporarily order the positions by amplitude and relabel them 1,2,3,41,2,3,4, with

σ1≥σ2≥σ3≥σ4. \sigma_1\ge\sigma_2\ge\sigma_3\ge\sigma_4.

This labels only amplitude order, without changing positions in the original ergodic average. Use the pair 1,21,2 in (Interpolated-count). Since there is at most one side position, at least one member of this pair is core.

By (Role-total), the worst amplitude cost from M′2ϑp0M'^{2\vartheta p_0} is bounded by

σ4−4ϑp0 \sigma_4^{-4\vartheta p_0}

The core member of the pair can also use (Core-cap), giving the factor

min⁡(1,D∗σi2)1−ϑ \min(1,D_*\sigma_i^2)^{1-\vartheta}

If that core position is i=2i=2, then σ2≤σ1\sigma_2\le\sigma_1 allows the same bound with σ1\sigma_1. Constants and powers of PP are absorbed into PCP^C.

Multiply by the pp-th power of the amplitude factor in (Cell-core) to obtain

PCmin⁡(1,D∗σ12)1−ϑσ1p−2(1−ϑ)σ2p−2(1−ϑ)σ3pσ4p−4ϑp0.(Amplitude) P^C \min(1,D_*\sigma_1^2)^{1-\vartheta} \sigma_1^{p-2(1-\vartheta)} \sigma_2^{p-2(1-\vartheta)} \sigma_3^p \sigma_4^{p-4\vartheta p_0}. \tag{Amplitude}

Denote the four exponents by e1,e2,e3,e4e_1,e_2,e_3,e_4. Substitution of p=1−ϑ+ϑp0p=1-\vartheta+\vartheta p_0 gives

e1+e2+e3+e4=0, e_1+e_2+e_3+e_4=0,

and

e1=−1+ϑ(1+p0),e1+e2=−2+2ϑ(1+p0),e1+e2+e3=−1+ϑ(1+3p0).(Partial-exponents) \begin{aligned} e_1&=-1+\vartheta(1+p_0),\\ e_1+e_2&=-2+2\vartheta(1+p_0),\\ e_1+e_2+e_3&=-1+\vartheta(1+3p_0). \end{aligned} \tag{Partial-exponents}

A sufficiently small fixed ϑ\vartheta makes all three values strictly negative.

Set

gj=log⁡2(σj/σj+1)∈Z≥0,j=1,2,3. g_j=\log_2(\sigma_j/\sigma_{j+1})\in\mathbb Z_{\ge0}, \qquad j=1,2,3.

Since the total exponent is zero,

∏i=14σiei=2 g1e1+g2(e1+e2)+g3(e1+e2+e3). \prod_{i=1}^4\sigma_i^{e_i} = 2^{\,g_1e_1+g_2(e_1+e_2)+g_3(e_1+e_2+e_3)}.

Each amplitude gap gjg_j therefore contributes a convergent geometric series.

It remains to sum over simultaneous multiplication of all amplitudes by one dyadic factor. On retained cells, σ1≤PC\sigma_1\le P^C. When

σ1<D∗−1/2 \sigma_1<D_*^{-1/2}

the prefactor in (Amplitude) is

(D∗σ12)1−ϑ, (D_*\sigma_1^2)^{1-\vartheta},

and decays geometrically as σ1\sigma_1 decreases dyadically. In the range D∗−1/2≤σ1≤PCD_*^{-1/2}\le\sigma_1\le P^C, there are only

O(1+log⁡D∗+log⁡P) O(1+\log D_*+\log P)

dyadic amplitudes. The common-scale cost is therefore only the permitted logarithmic polynomial. Finally sum over at most 2424 amplitude orderings.

9. Frequency summation and the order of choices

The frequency loss in (Count-one) is only a fixed power of 1+log⁡(ν/μ)1+\log(\nu/\mu). After interpolation, the second count costs at most

μ−CϑνCϑΛCϑ. \mu^{-C\vartheta}\nu^{C\vartheta}\Lambda^{C\vartheta}.

The pp-th power of the kernel coefficient is

μpν−LpΛ−Lp. \mu^p\nu^{-Lp}\Lambda^{-Lp}.

First choose the absolute parameter ϑ\vartheta sufficiently small that

p>2/3,p−Cϑ>0 p>2/3,\qquad p-C\vartheta>0

and all three strict negative inequalities in (Partial-exponents) hold. Then choose a sufficiently large fixed integer LL so that

Lp−Cϑ>0. Lp-C\vartheta>0.

We then have

∑μ=2−a, a≥0∑ν=2b, b≥0∑Λ=2c, c≥0μp−Cϑν−Lp+CϑΛ−Lp+Cϑ(1+log⁡(ν/μ))C<∞. \sum_{\mu=2^{-a},\,a\ge0} \sum_{\nu=2^b,\,b\ge0} \sum_{\Lambda=2^c,\,c\ge0} \mu^{p-C\vartheta} \nu^{-Lp+C\vartheta} \Lambda^{-Lp+C\vartheta} (1+\log(\nu/\mu))^C <\infty.

Strict geometric decay absorbs the fixed logarithmic power. Enlarging the actual finite frequency ranges to these infinite ranges only increases the bound.

The numbers of heights, types, position patterns, and retained search leaves are absorbed into a fixed power of PP. Thus, on every retained path,

∑G,sother configurations[CLμν−LΛ−L(∏jσj)NsG]p≤CqPC4.(Path-power) \sum_{\substack{G,s\\\text{other configurations}}} \left[ C_L\mu\nu^{-L}\Lambda^{-L} \left(\prod_j\sigma_j\right)N_s^G \right]^p \le C_qP^{C_4}. \tag{Path-power}

The parameters p0,ϑ,ε,C4p_0,\vartheta,\varepsilon,C_4 can all be fixed before deciding how close qq must be to two.

10. Returning to the minimum on each original interval

Let CIC_I be the sum of the absolute main contributions on an original cell. First take the cell's minimum, then use subadditivity for 0<p<10<p<1:

min⁡(η,CI)≤η1−pCIp≤ηε∑groups and configurations(full main contribution on I for this group and configuration)p.(Cell-minimum) \min(\eta,C_I) \le\eta^{1-p}C_I^p \le\eta^\varepsilon \sum_{\text{groups and configurations}} (\text{full main contribution on }I\text{ for this group and configuration})^p. \tag{Cell-minimum}

The sum may be split across groups and configurations, but each term's NsGN_s^G must remain intact. Splitting earlier into unit contributions from individual label tuples would lose the gain in (Count-small-power).

For nonnegative cell data FIF_I, finite summation and integration give the exact identity

∑I⊆R∣I∣FI=∫R∑I∋x∗FI dx∗. \sum_{I\subseteq R}|I|F_I = \int_R\sum_{I\ni x_*}F_I\,\mathrm dx_*.

Inserting (Path-power) yields

∑I retained∣I∣min⁡(η,sum of absolute core main contributions)≤CqηεPC4∣R∣. \sum_{I\text{ retained}}|I| \min(\eta,\text{sum of absolute core main contributions}) \le C_q\eta^\varepsilon P^{C_4}|R|.

Add the errors previously controlled separately in absolute value to obtain D (6.24):

CqηεPC4∣R∣+O(e−k∣R∣),1−ε>2/3.(Core-bound) C_q\eta^\varepsilon P^{C_4}|R| +O(e^{-k}|R|), \qquad 1-\varepsilon>2/3. \tag{Core-bound}

Source coverage and remaining work

  • D pp.57–58: the three checks for applying the core count to varying functions, and equations (6.23)–(6.24).
  • H §§9.1–9.2, pp.78–81: common heights, complete-component selection, torus kernel calculations, and actual side-function windows. The results used are stated here; torus approximation and all Fourier errors are not fully reproved.
  • H Lemma 9.1, October 5, 2026 version, pp.81–87: the full hypotheses are stated here, and the combinatorial proof has been developed and independently reviewed in the extension. The source frequency gaps and height grouping required by D retain their own assumptions.
  • H Proposition 9.2, pp.87–88: pairwise uniqueness, Parseval for actual side functions, and the deduction of p0p_0-power counting from sparse mass.
  • H Proposition 9.3, pp.89–90: the group inequality, amplitude-gap sum, frequency sum, and cellwise minimum developed in full here.

The next part combines the three types of position patterns, handles reassignment of original intervals on restarts, and explains why H and D require the same q>2q>2. Only after these parameter choices is the local estimate independent of original tree depth.