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Unit 1: From oscillation estimates to pointwise convergence through all lengths

This unit studies §3 of C. Proposition 3.5 is taken as the specified analytic input, and the subsequent convergence argument is developed in detail. The source passages are Definition 3.1 (p.5), Proposition 3.5 (pp.8–9), Lemmas 3.6–3.9 (pp.9–12), and the proof of the main theorem at the end of §3 (pp.12–13).

1. The conclusion, reductions, and specified input

1.1 The conclusion to be deduced

Source: C Theorem 1.1, p.1.

Let (X,F,μ)(X,\mathcal F,\mu) be a probability space, and let TT be invertible, bimeasurable, probability-preserving, and mixing. Fix three pairwise distinct nonzero integers λ1,λ2,λ3\lambda_1,\lambda_2,\lambda_3 and functions f1,f2,f3∈L∞(μ)f_1,f_2,f_3\in L^\infty(\mu). The paper claims that

AN(x)=1N∑n=1N∏j=13fj(Tλjnx)⟶p,p=∏j=13∫Xfj dμ A_N(x)=\frac1N\sum_{n=1}^{N}\prod_{j=1}^{3}f_j(T^{\lambda_jn}x) \longrightarrow p, \quad p=\prod_{j=1}^{3}\int_X f_j\,\mathrm{d}\mu

almost everywhere, as NN runs through all positive integers.

This unit proves that the conclusion follows from the oscillation estimate below. In the paper, that estimate is deduced from C Theorem 2.2 and Lemmas 3.2–3.4. Those results, together with the relevant proofs in H and D, are left for later discussion.

1.2 Normalizing the slopes and functions

Source: the first paragraph of C §2.1, p.3, and the last paragraph of §3, p.13.

Set

g=gcd⁡(∣λ1∣,∣λ2∣,∣λ3∣),S=Tg,bj=λj/g,b0=0. g=\gcd(|\lambda_1|,|\lambda_2|,|\lambda_3|), \quad S=T^g, \quad b_j=\lambda_j/g, \quad b_0=0.

Then b0,b1,b2,b3b_0,b_1,b_2,b_3 are pairwise distinct and gcd⁡(∣b1∣,∣b2∣,∣b3∣)=1\gcd(|b_1|,|b_2|,|b_3|)=1. Moreover, Tλjn=SbjnT^{\lambda_jn}=S^{b_jn}, so the averages are unchanged. The transformation SS remains invertible and probability-preserving. If TT is mixing, then SS is mixing, since ∣gn∣→∞|gn|\to\infty.

If some fjf_j has L∞L^\infty norm zero, choose the zero representative; the conclusion is immediate. Otherwise, divide each function by its norm. We first use measurable representatives satisfying ∣fj∣≤1|f_j|\le1 everywhere and restore the constant factors at the end.

The choice of representatives does not change an almost-everywhere conclusion. If fjf_j and f~j\widetilde f_j differ only on a null set ZjZ_j, all discrepancies at integer times lie in

Z=⋃j=13⋃m∈ZT−mZj. Z=\bigcup_{j=1}^{3}\bigcup_{m\in\mathbb Z}T^{-m}Z_j.

This is a measurable, TT-invariant null set. We may therefore work with everywhere bounded representatives without assuming completeness of the probability space.

Write

Fn(x)=∏j=13fj(Sbjnx),n∈Z. F_n(x)=\prod_{j=1}^{3}f_j(S^{b_jn}x), \quad n\in\mathbb Z.

Then ∣Fn(x)∣≤1|F_n(x)|\le1. The analytic input below requires only that SS be invertible and measure-preserving. Mixing enters when the limit is identified.

1.3 The precise class of smooth weights

Source: C Definition 3.1, p.5, equations (3.1)–(3.2).

A real-valued function φ\varphi is called an averaging weight here if φ∈Cc∞(R)\varphi\in C_c^\infty(\mathbb R),

∫Rφ(t) dt=1,∫Rtjφ(t) dt=0(j=1,2,3), \int_{\mathbb R}\varphi(t)\,\mathrm{d}t=1, \quad \int_{\mathbb R}t^j\varphi(t)\,\mathrm{d}t=0 \quad (j=1,2,3),

and there is a constant G≥1G\ge1 such that, for every integer r≥0r\ge0,

∥φ(r)∥∞≤[G(r+2)]G(r+2). \|\varphi^{(r)}\|_\infty \le [G(r+2)]^{G(r+2)}.

The constant GG may depend on φ\varphi. Different approximating weights below may require different values of GG. No uniform control of their supports or derivatives is asserted.

Such a weight φ\varphi must change sign. If φ≥0\varphi\ge0, the vanishing second moment would imply t2φ(t)=0t^2\varphi(t)=0 almost everywhere. Thus φ\varphi would be supported almost everywhere on the single point 00, contradicting its integral being 11. It cannot be interpreted as a nonnegative probability density.

Define

φa(t)=a−1φ(t/a),Vkφ(x)=∑n∈Zφ2k(n)Fn(x),k≥0. \varphi_a(t)=a^{-1}\varphi(t/a), \quad V_k^\varphi(x)=\sum_{n\in\mathbb Z}\varphi_{2^k}(n)F_n(x), \quad k\ge0.

If supp⁡φ⊆[−B,B]\operatorname{supp}\varphi\subseteq[-B,B], with B≥1B\ge1, each sum is finite and

∣Vkφ(x)∣≤2−k(2B2k+1)∥φ∥∞≤(2B+1)∥φ∥∞. |V_k^\varphi(x)| \le 2^{-k}(2B2^k+1)\|\varphi\|_\infty \le (2B+1)\|\varphi\|_\infty.

This is the uniform bound in C (3.10). It applies to one fixed weight; no common bound for all weights is required.

1.4 Proposition 3.5: The assumed oscillation estimate

Source: the statement at the end of C p.8 and its proof on p.9; the conclusion is equation (3.11).

Fix the slopes above and one averaging weight φ\varphi. The paper claims that there is a constant Cφ,b<∞C_{\varphi,b}\lt\infty such that, for every integer w≥1w\ge1 and every deterministic sequence of integer endpoints

0≤k1<k2<⋯<kw+1 0\le k_1\lt k_2\lt\cdots\lt k_{w+1}

we have

∑i=1w∫Xmax⁡ki≤ℓ≤ki+1∣Vℓφ(x)−Vkiφ(x)∣ dμ(x)≤Cφ,bw.(O) \sum_{i=1}^{w} \int_X \max_{k_i\le\ell\le k_{i+1}} |V_\ell^\varphi(x)-V_{k_i}^\varphi(x)| \,\mathrm{d}\mu(x) \le C_{\varphi,b}\sqrt w. \tag{O}

Here SS need only be invertible, bimeasurable, and probability-preserving; neither ergodicity nor mixing is required. The functions are normalized by ∣fj∣≤1|f_j|\le1. The constant may depend on the fixed slopes and weight, but not on the system, functions, endpoints, or number of blocks ww.

“Deterministic endpoints” means that the same kik_i are used for every xx. The maximizing position may depend on xx, but each maximum is taken over finitely many scales, so its integrand is measurable. These two facts are compatible.

Estimate (O) is not treated here as an established classical theorem. It is the crucial input claimed by the manuscript and still to be verified. Its stated derivation runs through the local depth-varying estimate C Theorem 2.2 (pp.3–4), the cancellation kernel in C Lemma 3.2 (p.6), the real-line estimate C Lemma 3.3 (p.7), the integer-sequence estimate C Lemma 3.4 (pp.7–8), and finally finite-orbit transference.

2. Why oscillation rules out nonconvergence on a set of positive measure

Source: C Lemma 3.6, pp.9–10. We first formulate the assertion for an abstract sequence of functions.

2.1 The full statement

Let (Zk)k≥0(Z_k)_{k\ge0} be a uniformly bounded sequence of measurable complex-valued functions on a probability space. Suppose there is a constant CC such that, for every w≥1w\ge1 and every deterministic sequence of endpoints 0≤k1<⋯<kw+10\le k_1\lt\cdots\lt k_{w+1},

∑i=1w∫Xmax⁡ki≤ℓ≤ki+1∣Zℓ−Zki∣ dμ≤Cw. \sum_{i=1}^{w}\int_X \max_{k_i\le\ell\le k_{i+1}} |Z_\ell-Z_{k_i}|\,\mathrm{d}\mu \le C\sqrt w.

Then Zk(x)Z_k(x) converges on a measurable set of full measure. The conclusion specifies neither the limit nor a rate of convergence.

2.2 Tail diameters and a fixed amplitude

Source: p.9, the first paragraph in the proof of Lemma 3.6 and the tail-diameter formula.

Set

ωK(x)=sup⁡p,q≥K∣Zp(x)−Zq(x)∣,ω(x)=lim⁡K→∞ωK(x). \omega_K(x)=\sup_{p,q\ge K}|Z_p(x)-Z_q(x)|, \quad \omega(x)=\lim_{K\to\infty}\omega_K(x).

Each supremum involves only countably many measurable functions, so ωK\omega_K is measurable. It decreases with KK and is finite by uniform boundedness; hence its limit exists and is measurable. The condition ω(x)=0\omega(x)=0 is equivalent to (Zk(x))(Z_k(x)) being Cauchy. By completeness of the complex numbers, this is also equivalent to convergence.

Suppose, to the contrary, that μ{ω>0}>0\mu\{\omega>0\}>0. Since

{ω>0}=⋃m=1∞{ω>2/m}, \{\omega>0\}=\bigcup_{m=1}^{\infty}\{\omega>2/m\},

some mm yields a set of positive measure on the right. Write δ=1/m\delta=1/m and

E={ω>2δ},d=μ(E)>0. E=\{\omega>2\delta\}, \quad d=\mu(E)>0.

From now on, E,d,δE,d,\delta are fixed. Individual points may originally have different tail amplitudes; this choice restricts them to a common positive amplitude.

2.3 A deterministic finite block from an infinite tail

Source: p.10, the opening of the proof of Lemma 3.6, immediately after the definition of EE.

Fix any integer K≥0K\ge0. For p,q≥Kp,q\ge K, the triangle inequality implies

∣Zp−Zq∣≤∣Zp−ZK∣+∣Zq−ZK∣. |Z_p-Z_q|\le |Z_p-Z_K|+|Z_q-Z_K|.

Taking suprema, we obtain

sup⁡ℓ≥K∣Zℓ−ZK∣≥12ωK≥12ω>δon E. \sup_{\ell\ge K}|Z_\ell-Z_K| \ge\frac12\omega_K \ge\frac12\omega >\delta \quad\text{on }E\text{.}

Set

MK,L(x)=max⁡K≤ℓ≤L∣Zℓ(x)−ZK(x)∣. M_{K,L}(x)=\max_{K\le\ell\le L}|Z_\ell(x)-Z_K(x)|.

As L→∞L\to\infty, the quantities MK,LM_{K,L} increase to the tail supremum above. The monotone convergence theorem implies

lim⁡L→∞∫XMK,L dμ≥δd. \lim_{L\to\infty}\int_XM_{K,L}\,\mathrm{d}\mu \ge\delta d.

There is therefore a deterministic integer L>KL>K such that

∫XMK,L dμ≥δd/2.(B) \int_XM_{K,L}\,\mathrm{d}\mu\ge\delta d/2. \tag{B}

The integer LL is chosen using the integral; it is not a function of xx. Estimate (B) does not require every point of EE to make an excursion within this block, or require the excursions to occur at the same scale. It only requires the integral of the block maximum to reach a fixed positive value.

2.4 Linear lower growth versus a square-root upper bound

Source: p.10, the last three sentences of the proof of Lemma 3.6.

Start with k1=0k_1=0. At each step, use the previous endpoint as the new KK and choose the next endpoint by (B). This produces deterministic, strictly increasing endpoints, with the same lower bound δd/2\delta d/2 on every block. Consequently, for every ww,

wδd2≤∑i=1w∫Xmax⁡ki≤ℓ≤ki+1∣Zℓ−Zki∣ dμ≤Cw. \frac{w\delta d}{2} \le\sum_{i=1}^{w}\int_X \max_{k_i\le\ell\le k_{i+1}}|Z_\ell-Z_{k_i}| \,\mathrm{d}\mu \le C\sqrt w.

Thus w≤2C/(δd)\sqrt w\le2C/(\delta d). The right side is fixed, whereas ww can be arbitrarily large, a contradiction. Hence ω=0\omega=0 almost everywhere, which proves the assertion.

Apply this to Zk=VkφZ_k=V_k^\varphi, using (O) and the uniform bound from §1.3. The smooth averages for each fixed weight converge almost everywhere. Mixing has not been used.

2.5 Why sublinear growth matters

A bound of only CwCw would not suffice. For example, Zk(x)=(−1)kZ_k(x)=(-1)^k is independent of xx. Its maximal oscillation on each integer block with distinct endpoints is 22, so the total is 2w2w, but the sequence does not converge. What matters is sublinear growth uniformly over all choices of endpoints.

Even if each point continues to make excursions, no single excursion time need work for every point. Taking a finite maximum before integrating avoids this error in the order of quantifiers.

3. Multiple L2L^2 convergence from ordinary mixing

Source: C Lemmas 3.7–3.8, pp.10–11. We state the norm-convergence theorem for any finite number of factors. In the present triple-average application, the transformation is SS.

Let (X,F,μ)(X,\mathcal F,\mu) be a probability space, and let TT be invertible, bimeasurable, probability-preserving, and mixing. Fix an integer d≥1d\ge1, pairwise distinct nonzero integers a1,…,ada_1,\ldots,a_d, and functions f1,…,fd∈L∞(μ)f_1,\ldots,f_d\in L^\infty(\mu). Then

1N∑n=1N∏j=1dfj∘Tajn⟶∏j=1d∫Xfj dμin L2(μ). \frac1N\sum_{n=1}^N\prod_{j=1}^d f_j\circ T^{a_jn} \longrightarrow\prod_{j=1}^d\int_Xf_j\,\mathrm{d}\mu \quad\text{in }L^2(\mu).

This is a norm-convergence statement. It does not directly yield almost-everywhere convergence through all lengths, and it is distinct from higher-order mixing without time averaging.

3.1 From mixing of sets to correlations of functions

Source: C p.10, the beginning of §3.3 and equation (3.13).

Mixing of sets asserts that, for fixed E,F∈FE,F\in\mathcal F, we have μ(E∩T−mF)→μ(E)μ(F)\mu(E\cap T^{-m}F)\to\mu(E)\mu(F) as ∣m∣→∞|m|\to\infty. We need to deduce that, for fixed bounded measurable functions g,hg,h,

∫Xg(h∘Tm) dμ⟶(∫Xg dμ)(∫Xh dμ). \int_Xg(h\circ T^m)\,\mathrm{d}\mu \longrightarrow \left(\int_Xg\,\mathrm{d}\mu\right) \left(\int_Xh\,\mathrm{d}\mu\right).

If g,hg,h are simple functions, express them as finite linear combinations of indicator functions. The integral on the left expands into finitely many set correlations, and the conclusion follows term by term from the definition.

In general, for each ε>0\varepsilon>0, choose simple functions gε,hεg_\varepsilon,h_\varepsilon with ∥g−gε∥∞≤ε\|g-g_\varepsilon\|_\infty\le\varepsilon and ∥h−hε∥∞≤ε\|h-h_\varepsilon\|_\infty\le\varepsilon. Such uniform approximations follow by dividing the bounded complex ranges into finitely many small cells. For every mm,

∣∫gh∘Tm−∫gεhε∘Tm∣≤ε∥h∥∞+(∥g∥∞+ε)ε. \left|\int gh\circ T^m-\int g_\varepsilon h_\varepsilon\circ T^m\right| \le\varepsilon\|h\|_\infty+(\|g\|_\infty+\varepsilon)\varepsilon.

The difference between the corresponding products of integrals has the same upper bound. Fix ε\varepsilon, apply the simple-function conclusion as ∣m∣→∞|m|\to\infty, and then let ε↓0\varepsilon\downarrow0. This proves the required function formulation. Complex coefficients cause no change in the argument.

3.2 Lemma 3.7: A finite Hilbert-space inequality

Source: C p.10, the proof from the zero-extension identity through the estimate for finite HH.

Let vnv_n belong to a Hilbert space, with ∥vn∥≤M\|v_n\|\le M. Suppose that, for every fixed positive integer hh, the limit

γh=lim⁡N→∞1N∑n=1N−h⟨vn+h,vn⟩ \gamma_h=\lim_{N\to\infty}\frac1N\sum_{n=1}^{N-h}\langle v_{n+h},v_n\rangle

exists. The inner product is taken to be linear in the first variable. For each fixed integer H≥1H\ge1, we have

lim sup⁡N→∞∥1N∑n=1Nvn∥2≤M2H+2H2∑h=1H−1(H−h)∣γh∣.(H) \limsup_{N\to\infty}\left\|\frac1N\sum_{n=1}^Nv_n\right\|^2 \le\frac{M^2}{H}+\frac{2}{H^2}\sum_{h=1}^{H-1}(H-h)|\gamma_h|. \tag{H}

To prove this, fix HH and take N≥HN\ge H. For this finite estimate only, extend the sequence outside 1≤n≤N1\le n\le N by setting vnv_n to zero. Then

H∑n=1Nvn=∑r=1N+H∑j=0H−1vr−j. H\sum_{n=1}^Nv_n=\sum_{r=1}^{N+H}\sum_{j=0}^{H-1}v_{r-j}.

By the Cauchy–Schwarz inequality,

∥1N∑n=1Nvn∥2≤N+HH2N2∑r=1N+H∥∑j=0H−1vr−j∥2. \left\|\frac1N\sum_{n=1}^Nv_n\right\|^2 \le\frac{N+H}{H^2N^2} \sum_{r=1}^{N+H}\left\|\sum_{j=0}^{H-1}v_{r-j}\right\|^2.

Expand the square on the right. The diagonal terms sum to at most HNM2HNM^2, and the terms with displacement hh occur H−hH-h times. Thus

∑r=1N+H∥∑j=0H−1vr−j∥2=H∑n=1N∥vn∥2+2Re⁡∑h=1H−1(H−h)∑n=1N−h⟨vn+h,vn⟩. \begin{aligned} \sum_{r=1}^{N+H}\left\|\sum_{j=0}^{H-1}v_{r-j}\right\|^2 &=H\sum_{n=1}^N\|v_n\|^2\\ &\quad+2\operatorname{Re}\sum_{h=1}^{H-1}(H-h) \sum_{n=1}^{N-h}\langle v_{n+h},v_n\rangle. \end{aligned}

With HH fixed, let N→∞N\to\infty to obtain (H). If γh→0\gamma_h\to0, then

2H2∑h=1H−1(H−h)∣γh∣≤2H∑h=1H−1∣γh∣⟶0. \frac{2}{H^2}\sum_{h=1}^{H-1}(H-h)|\gamma_h| \le\frac2H\sum_{h=1}^{H-1}|\gamma_h|\longrightarrow0.

Letting H→∞H\to\infty now shows that the average vectors converge to zero in norm.

3.3 Lemma 3.8: Induction on the number of factors

Source: C p.11, the proof of (3.14), ending with the expansion after subtracting means.

First consider the case in which at least one function has mean zero. Set

vn=∏j=1dfj∘Tajn,qj,h=(fj∘Tajh)fj‾. v_n=\prod_{j=1}^df_j\circ T^{a_jn},\quad q_{j,h}=(f_j\circ T^{a_jh})\overline{f_j}.

For fixed hh, invariance of the measure implies

⟨vn+h,vn⟩=∫Xq1,h(x)∏j=2dqj,h(T(aj−a1)nx) dμ(x).(C) \langle v_{n+h},v_n\rangle =\int_Xq_{1,h}(x)\prod_{j=2}^dq_{j,h}(T^{(a_j-a_1)n}x)\,\mathrm{d}\mu(x). \tag{C}

If d=1d=1, the right side is independent of nn, so γh=∫Xq1,h dμ\gamma_h=\int_Xq_{1,h}\,\mathrm{d}\mu.

Suppose the theorem holds for d−1d-1 functions. The slopes aj−a1a_j-a_1, for 2≤j≤d2\le j\le d, are pairwise distinct and nonzero. The induction hypothesis therefore implies

1N∑n=1N∏j=2dqj,h∘T(aj−a1)n⟶∏j=2d∫Xqj,h dμin L2. \frac1N\sum_{n=1}^N\prod_{j=2}^dq_{j,h}\circ T^{(a_j-a_1)n} \longrightarrow\prod_{j=2}^d\int_Xq_{j,h}\,\mathrm{d}\mu \quad\text{in }L^2.

Denote the left side by GN,hG_{N,h} and its constant limit by chc_h. Since q1,h∈L2(μ)q_{1,h}\in L^2(\mu), the Cauchy–Schwarz inequality implies

∣∫Xq1,h(GN,h−ch) dμ∣≤∥q1,h∥2 ∥GN,h−ch∥2⟶0. \left|\int_X q_{1,h}(G_{N,h}-c_h)\,\mathrm{d}\mu\right| \le \|q_{1,h}\|_2\,\|G_{N,h}-c_h\|_2\longrightarrow0.

Insert this limit into (C). For fixed hh, deleting the final hh terms introduces an error of O(h/N)O(h/N). We obtain

γh=∏j=1d∫Xqj,h dμ. \gamma_h=\prod_{j=1}^d\int_Xq_{j,h}\,\mathrm{d}\mu.

Since aj≠0a_j\ne0, mixing implies

∫Xqj,h dμ⟶∣∫Xfj dμ∣2(h→∞). \int_Xq_{j,h}\,\mathrm{d}\mu \longrightarrow\left|\int_Xf_j\,\mathrm{d}\mu\right|^2 \quad(h\to\infty).

At least one fjf_j has mean zero, so γh→0\gamma_h\to0. By (H), we have N−1∑n=1Nvn→0N^{-1}\sum_{n=1}^Nv_n\to0 in L2L^2.

Finally, write each function as

fj=mj+(fj−mj),mj=∫Xfj dμ. f_j=m_j+(f_j-m_j),\quad m_j=\int_Xf_j\,\mathrm{d}\mu.

Expand the product. The term consisting entirely of constants is ∏jmj\prod_jm_j. Every other term contains at least one mean-zero function, and there are only finitely many such terms. Their averages therefore tend to zero in L2L^2. This completes the induction.

3.4 Assumptions and order of limits

  • Distinct slopes ensure that the difference slopes in the induction are nonzero.
  • Each slope is nonzero, so ∣ajh∣→∞|a_jh|\to\infty and mixing applies.
  • Invertibility permits negative times and the measure-preserving change of variables.
  • Boundedness places every product in L2L^2 and controls the finitely many terms deleted for fixed hh.
  • First fix hh, then let N→∞N\to\infty. In (H), first fix HH and only at the end let H→∞H\to\infty. No rate of mixing is needed.

The slope conditions cannot be dropped. For instance, with two equal slopes and f2=f1‾f_2=\overline{f_1}, the average is an ordinary ergodic average of ∣f1∣2|f_1|^2, whose limit is generally not ∣∫f1∣2|\int f_1|^2. If a zero slope is allowed and the other function is identically one, the zero-slope observable retains its dependence on the starting point.

4. Smooth weighted L2L^2 convergence and identification of the pointwise limit

Source: C Lemma 3.8, p.11, from the positive- and negative-time partial sums through (3.15), followed by the Fatou argument.

4.1 Positive and negative times must be treated separately

Return to the notation Fn=∏j=13fj∘SbjnF_n=\prod_{j=1}^{3}f_j\circ S^{b_jn} and p=∏j∫fj dμp=\prod_j\int f_j\,\mathrm{d}\mu from §1. Apply the norm-convergence theorem separately to the slopes bjb_j and −bj-b_j. This yields

RN±=∑n=1N(F±n−p),∥RN±∥2=o(N). R_N^\pm=\sum_{n=1}^{N}(F_{\pm n}-p), \quad \|R_N^\pm\|_2=o(N).

Both sets of slopes are pairwise distinct and nonzero, so both applications are valid. Negative times cannot be omitted here, since the averaging weight may have support on the negative half-line.

More generally, fix any χ∈Cc1(R)\chi\in C_c^1(\mathbb R) with ∫χ=1\int\chi=1. We will prove that

∑n∈Za−1χ(n/a)Fn⟶pin L2(μ),a⟶∞.(W) \sum_{n\in\mathbb Z}a^{-1}\chi(n/a)F_n \longrightarrow p \quad\text{in }L^2(\mu), \quad a\longrightarrow\infty. \tag{W}

This conclusion requires neither the first three moments to vanish nor the higher-derivative bounds of §1.3. Those two conditions belong to the smaller class of weights used for the oscillation estimate.

4.2 The finite summation-by-parts identity

Choose B≥1B\ge1 such that supp⁡χ⊆[−B,B]\operatorname{supp}\chi\subseteq[-B,B]. Set

Ma=⌊Ba⌋+1,wn±=a−1χ(±n/a). M_a=\lfloor Ba\rfloor+1, \quad w_n^\pm=a^{-1}\chi(\pm n/a).

Since Ma/a>BM_a/a>B, we have wMa±=0w_{M_a}^\pm=0, and all subsequent weights also vanish. With the convention R0±=0R_0^\pm=0,

F±n−p=Rn±−Rn−1±. F_{\pm n}-p=R_n^\pm-R_{n-1}^\pm.

Expanding the terms and shifting indices yields the exact identity

∑n=1Mawn±(F±n−p)=∑n=1Mawn±(Rn±−Rn−1±)=∑n=1Ma−1(wn±−wn+1±)Rn±. \begin{aligned} \sum_{n=1}^{M_a}w_n^\pm(F_{\pm n}-p) &=\sum_{n=1}^{M_a}w_n^\pm(R_n^\pm-R_{n-1}^\pm)\\ &=\sum_{n=1}^{M_a-1}(w_n^\pm-w_{n+1}^\pm)R_n^\pm. \end{aligned}

The terminal term wMa±RMa±w_{M_a}^\pm R_{M_a}^\pm vanishes, and the initial term contains R0±=0R_0^\pm=0, so there are no remaining boundary terms.

By the mean value theorem,

∣wn±−wn+1±∣≤a−2∥χ′∥∞. |w_n^\pm-w_{n+1}^\pm| \le a^{-2}\|\chi'\|_\infty.

Thus the positive- and negative-time parts each satisfy

∥∑n=1Mawn±(F±n−p)∥2≤a−2∥χ′∥∞∑n=1Ma−1∥Rn±∥2.(A) \left\|\sum_{n=1}^{M_a}w_n^\pm(F_{\pm n}-p)\right\|_2 \le a^{-2}\|\chi'\|_\infty \sum_{n=1}^{M_a-1}\|R_n^\pm\|_2. \tag{A}

4.3 Why the bound is o(1)o(1)

Given ε>0\varepsilon>0, first choose a fixed N0N_0 such that, for both signs and every n≥N0n\ge N_0, we have ∥Rn±∥2≤εn\|R_n^\pm\|_2\le\varepsilon n. This is the only use of the o(N)o(N) estimate.

Split the right side of (A) into n<N0n<N_0 and n≥N0n\ge N_0. The first part is a fixed finite sum multiplied by a−2a^{-2}, so it tends to zero as a→∞a\to\infty. The second part is at most

εa−2∥χ′∥∞∑n=1Ma−1n≤ε2∥χ′∥∞Ma2a2. \varepsilon a^{-2}\|\chi'\|_\infty\sum_{n=1}^{M_a-1}n \le\frac{\varepsilon}{2}\|\chi'\|_\infty \frac{M_a^2}{a^2}.

Since Ma/a→BM_a/a\to B, its limit superior is at most εB2∥χ′∥∞/2\varepsilon B^2\|\chi'\|_\infty/2. Finally let ε↓0\varepsilon\downarrow0. Both weighted errors tend to zero. No rate of decay of ∥Rn±∥2/n\|R_n^\pm\|_2/n has been assumed.

The centered term at n=0n=0 is a−1χ(0)(F0−p)a^{-1}\chi(0)(F_0-p), whose L2L^2 norm is O(a−1)O(a^{-1}). The constant part satisfies

p a−1∑n∈Zχ(n/a)⟶p∫Rχ(t) dt=p p\,a^{-1}\sum_{n\in\mathbb Z}\chi(n/a)\longrightarrow p\int_{\mathbb R}\chi(t)\,\mathrm{d}t=p

because χ\chi is continuous and compactly supported, and its uniform-grid Riemann sums converge. Combining the three parts proves (W).

4.4 Identifying the existing pointwise limit

Take χ=φ\chi=\varphi and a=2ka=2^k. Then Vkφ→pV_k^\varphi\to p in L2L^2. Section 2 already shows that VkφV_k^\varphi converges on a measurable full-measure set EφE_\varphi; denote its limit by LφL_\varphi. Fatou's lemma implies

∫Eφ∣Lφ−p∣2 dμ≤lim inf⁡k→∞∫Eφ∣Vkφ−p∣2 dμ≤lim inf⁡k→∞∥Vkφ−p∥22=0. \int_{E_\varphi}|L_\varphi-p|^2\,\mathrm{d}\mu \le\liminf_{k\to\infty} \int_{E_\varphi}|V_k^\varphi-p|^2\,\mathrm{d}\mu \le\liminf_{k\to\infty}\|V_k^\varphi-p\|_2^2=0.

Hence Lφ=pL_\varphi=p almost everywhere. If necessary, remove one more measurable null set from EφE_\varphi so that Vkφ(x)→pV_k^\varphi(x)\to p for every x∈Eφx\in E_\varphi.

Dominated convergence is not needed to obtain the integral conclusion; Fatou's lemma suffices. Mixing establishes the norm limit in this section, while the oscillation estimate established the existence of the pointwise limit through all scales.

5. Smooth weights: derivative bounds and approximation with vanishing moments

Source: the smooth-function construction following C Definition 3.1, p.5, and Lemma 3.9, p.12. These passages address the derivative condition and the moment correction, respectively.

5.1 A nonnegative smooth function with the required derivative growth

Set

ρ0(t)={exp⁡ ⁣(−1/(1−t2)),∣t∣<1,0,∣t∣≥1. \rho_0(t)= \begin{cases} \exp\!\bigl(-1/(1-t^2)\bigr),&|t|\lt1,\\ 0,&|t|\ge1. \end{cases}

This function is smooth and positive on (−1,1)(-1,1). We must check that its zero extension is smooth at the endpoints and that all derivatives obey the growth condition of §1.3.

Fix ∣t∣<1|t|<1 and write d=1−t2d=1-t^2. In the complex plane, consider ∣z−t∣≤d/16|z-t|\le d/16. Then

∣(1−z2)−d∣=∣z−t∣ ∣z+t∣≤d16(2+116)<d4. |(1-z^2)-d| =|z-t|\,|z+t| \le\frac{d}{16}\left(2+\frac1{16}\right) <\frac d4.

Consequently, Re⁡(1−z2)≥3d/4\operatorname{Re}(1-z^2)\ge3d/4 and ∣1−z2∣≤5d/4|1-z^2|\le5d/4. Using Re⁡(1/q)=Re⁡(q)/∣q∣2\operatorname{Re}(1/q)=\operatorname{Re}(q)/|q|^2, we obtain

Re⁡11−z2≥1225d. \operatorname{Re}\frac1{1-z^2}\ge\frac{12}{25d}.

The denominator does not vanish in the disk, so exp⁡(−1/(1−z2))\exp(-1/(1-z^2)) is analytic there, with absolute value at most exp⁡(−12/(25d))\exp(-12/(25d)). The Cauchy derivative estimate therefore yields

∣ρ0(r)(t)∣≤r!(16d)rexp⁡ ⁣(−1225d).(G) |\rho_0^{(r)}(t)| \le r!\left(\frac{16}{d}\right)^r \exp\!\left(-\frac{12}{25d}\right). \tag{G}

For fixed rr, the right side tends to zero as d↓0d\downarrow0, since exponential decay dominates every fixed power. Each interior derivative extends continuously to zero at both endpoints. Checking the derivatives successively shows that the zero extension belongs to Cc∞(R)C_c^\infty(\mathbb R).

For a bound in terms of rr, set u=1/d≥1u=1/d\ge1. The maximum of ure−cuu^r\mathrm e^{-cu} on the positive half-line is (r/(ce))r(r/(c\mathrm e))^r; for r=0r=0, use a constant bound separately. By (G), there is an absolute constant CC such that

∥ρ0(r)∥∞≤Cr+1r!(r+1)r. \|\rho_0^{(r)}\|_\infty \le C^{r+1}r!(r+1)^r.

Since r!≤(r+1)rr!\le(r+1)^r, choosing a sufficiently large fixed GG bounds the right side by [G(r+2)]G(r+2)[G(r+2)]^{G(r+2)}. Normalize by setting

ρ=ρ0/∫Rρ0(t) dt \rho=\rho_0\left/\int_{\mathbb R}\rho_0(t)\,\mathrm{d}t\right.

Then ρ\rho is nonnegative, has mass 11, is supported in [−1,1][-1,1], and still satisfies a derivative bound of the same form.

The function ρ\rho is only an ingredient in constructing an averaging weight; it does not yet have the required vanishing moments. Its nonnegativity does not conflict with the fact that an averaging weight must change sign.

5.2 Stability of the derivative class under fixed operations

Source: C p.5, the paragraph on closure properties following Definition 3.1.

A fixed translation leaves the derivative supremum norms unchanged. For a fixed scale a>0a>0 and a fixed center zz,

drdtr[a−1ρ(t/a−z)]=a−r−1ρ(r)(t/a−z). \frac{\mathrm{d}^r}{\mathrm{d}t^r} \left[a^{-1}\rho(t/a-z)\right] =a^{-r-1}\rho^{(r)}(t/a-z).

A fixed dilation therefore introduces a factor growing at most exponentially in rr, which can be absorbed by increasing GG. Differentiation of a fixed order replaces rr by r+mr+m. A fixed finite linear combination adds only finitely many derivative bounds, again absorbed by increasing GG. The word “fixed” is important: no single GG has been obtained uniformly over all translation parameters, scales, or linear combinations.

5.3 The full statement of Lemma 3.9

For every c∈[1,2]c\in[1,2] and ε>0\varepsilon>0, there is an averaging weight φ\varphi in the sense of §1.3 such that

hc(t)=c−11(0,c](t),∥φ−hc∥L1(R)<ε. h_c(t)=c^{-1}\mathbf1_{(0,c]}(t), \quad \|\varphi-h_c\|_{L^1(\mathbb R)}<\varepsilon.

The weight φ\varphi must simultaneously have mass 11, vanishing first, second, and third moments, compact support, and the stated derivative growth. Density of Cc∞C_c^\infty in L1L^1 alone does not prove this assertion.

5.4 Smoothing the interval weight and fixing the initial moments

Source: C p.12, the first paragraph of the proof of Lemma 3.9.

Set ρδ(t)=δ−1ρ(t/δ)\rho_\delta(t)=\delta^{-1}\rho(t/\delta) and

v=hc∗ρδ. v=h_c*\rho_\delta.

The function vv is real-valued, nonnegative, smooth, and compactly supported, with ∫v=1\int v=1 and support contained in [−δ,c+δ][-\delta,c+\delta]. For any real ss, the symmetric difference of two length-cc intervals whose positions differ by that amount has length 2min⁡(∣s∣,c)2\min(|s|,c). Hence

∥hc( ⋅−s)−hc∥1=2min⁡(∣s∣,c)c. \|h_c(\,\cdot-s)-h_c\|_1 =\frac{2\min(|s|,c)}{c}.

By the integral triangle inequality and ρδ≥0\rho_\delta\ge0,

∥v−hc∥1≤∫Rρδ(s)∥hc( ⋅−s)−hc∥1 ds≤2δ/c. \begin{aligned} \|v-h_c\|_1 &\le\int_{\mathbb R}\rho_\delta(s) \|h_c(\,\cdot-s)-h_c\|_1\,\mathrm{d}s\\ &\le2\delta/c. \end{aligned}

Choose δ\delta small enough that ∥v−hc∥1<ε/2\|v-h_c\|_1<\varepsilon/2. Since ∥hc∥1=1\|h_c\|_1=1, we also have

∥v(r)∥∞≤∥ρδ(r)∥∞=δ−r−1∥ρ(r)∥∞. \|v^{(r)}\|_\infty \le\|\rho_\delta^{(r)}\|_\infty =\delta^{-r-1}\|\rho^{(r)}\|_\infty.

The preceding subsection shows that vv belongs to the required derivative class. Now fix vv and write

mj=∫Rtjv(t) dt,j=1,2,3. m_j=\int_{\mathbb R}t^jv(t)\,\mathrm{d}t, \quad j=1,2,3.

In general, mj≠0m_j\ne0, so these moments still need correction. Subsequent constants may depend on the function vv, which is now fixed.

5.5 Invertibility of the moment-correction matrix

Source: C p.12, the paragraph in the proof of Lemma 3.9 defining PjP_j, ρi,A\rho_{i,A}, and the matrix MM.

Fix four pairwise distinct real numbers z0,z1,z2,z3z_0,z_1,z_2,z_3, for example 0,1,2,30,1,2,3. Set

μr=∫Rurρ(u) du,μ0=1, \mu_r=\int_{\mathbb R}u^r\rho(u)\,\mathrm{d}u, \quad \mu_0=1,
Pj(z)=∫R(z+u)jρ(u) du=∑r=0j(jr)μrzj−r(0≤j≤3). P_j(z)=\int_{\mathbb R}(z+u)^j\rho(u)\,\mathrm{d}u =\sum_{r=0}^{j}\binom jr\mu_r z^{j-r} \quad (0\le j\le3).

Thus PjP_j is a monic polynomial of degree jj. Index the rows of the matrix by jj and the columns by ii, and set

M=(Pj(zi))0≤j,i≤3,V=(zij)0≤j,i≤3. M=(P_j(z_i))_{0\le j,i\le3}, \quad V=(z_i^j)_{0\le j,i\le3}.

If

Ljℓ={(jℓ)μj−ℓ,0≤ℓ≤j,0,ℓ>j, L_{j\ell}= \begin{cases} \binom j\ell\mu_{j-\ell},&0\le\ell\le j,\\ 0,&\ell>j, \end{cases}

then M=LVM=LV. The matrix LL is lower triangular, with every diagonal entry equal to μ0=1\mu_0=1. Thus

det⁡M=det⁡V=∏0≤i<ℓ≤3(zℓ−zi)≠0. \det M=\det V=\prod_{0\le i<\ell\le3}(z_\ell-z_i)\ne0.

This identity makes explicit the triangular change from a Vandermonde matrix mentioned in the paper. The matrix MM is now a fixed real invertible matrix.

5.6 Moving a small amount of mass to a large scale

For a scale A≥1A\ge1, define

ρi,A(t)=A−1ρ(t/A−zi). \rho_{i,A}(t)=A^{-1}\rho(t/A-z_i).

This is nonnegative and has mass 11. The substitution t=A(zi+u)t=A(z_i+u) yields

∫Rtjρi,A(t) dt=AjPj(zi). \int_{\mathbb R}t^j\rho_{i,A}(t)\,\mathrm{d}t =A^jP_j(z_i).

Solve the linear system

Mβ=(0−m1/A−m2/A2−m3/A3),β=(β0,β1,β2,β3)T. M\beta= \begin{pmatrix} 0\\-m_1/A\\-m_2/A^2\\-m_3/A^3 \end{pmatrix}, \quad \beta=(\beta_0,\beta_1,\beta_2,\beta_3)^{\mathsf T}.

Since A≥1A\ge1, the vector ℓ1\ell^1 norm satisfies

∑i=03∣βi∣≤∥M−1∥ℓ1→ℓ1(∣m1∣A+∣m2∣A2+∣m3∣A3)≤∥M−1∥ℓ1→ℓ1A∑j=13∣mj∣.(M) \sum_{i=0}^{3}|\beta_i| \le\|M^{-1}\|_{\ell^1\to\ell^1} \left(\frac{|m_1|}{A}+\frac{|m_2|}{A^2}+\frac{|m_3|}{A^3}\right) \le\frac{\|M^{-1}\|_{\ell^1\to\ell^1}}{A} \sum_{j=1}^{3}|m_j|. \tag{M}

Define

φ=v+∑i=03βiρi,A. \varphi=v+\sum_{i=0}^{3}\beta_i\rho_{i,A}.

Row zero of the system states that ∑iβi=0\sum_i\beta_i=0, so ∫φ=1\int\varphi=1. For j=1,2,3j=1,2,3, multiply row jj by AjA^j to obtain

∫Rtjφ(t) dt=mj+Aj∑i=03βiPj(zi)=0. \int_{\mathbb R}t^j\varphi(t)\,\mathrm{d}t =m_j+A^j\sum_{i=0}^{3}\beta_iP_j(z_i)=0.

Since each ρi,A\rho_{i,A} is nonnegative and has mass 11,

∥φ−v∥1≤∑i∣βi∣. \|\varphi-v\|_1\le\sum_i|\beta_i|.

Choose AA large enough that the right side of (M) is less than ε/2\varepsilon/2. Then

∥φ−hc∥1≤∥φ−v∥1+∥v−hc∥1<ε. \|\varphi-h_c\|_1 \le\|\varphi-v\|_1+\|v-h_c\|_1<\varepsilon.

All coefficients are real, and AA is now fixed. The weight φ\varphi is a finite sum of compactly supported smooth functions; §5.2 ensures the derivative growth condition. All requirements in the definition of an averaging weight have therefore been checked.

5.7 Why the expanding support matters

The support of ρi,A\rho_{i,A} lies in A[zi−1,zi+1]A[z_i-1,z_i+1]. Higher accuracy may require larger AA, and hence larger supports for the correction terms. Their L1L^1 mass is O(A−1)O(A^{-1}), whereas their jj-th moments may be amplified by AjA^j. A small L1L^1 change can therefore correct the low-order moments exactly.

If instead every approximant were required to be supported in the same interval [−R,R][-R,R], then

∣∫t2(φ−hc) dt∣≤R2∥φ−hc∥1 \left|\int t^2(\varphi-h_c)\,\mathrm{d}t\right| \le R^2\|\varphi-h_c\|_1

For R≥cR\ge c, this would force the second moments to converge as the L1L^1 error tends to zero. But ∫t2φ=0\int t^2\varphi=0, whereas ∫t2hc=c2/3>0\int t^2h_c=c^2/3>0, a contradiction. A common fixed support cannot be added to the approximation statement. The paper does not impose one.

6. From smooth dyadic scales to all integer lengths

Source: C pp.12–13, the proof of the main theorem following Lemma 3.9, especially (3.16)–(3.17) and the finite rational grid on p.13.

6.1 One countable intersection of full-measure sets

For each rational c∈[1,2]c\in[1,2] and each integer h≥1h\ge1, choose in advance an averaging weight φc,h\varphi_{c,h} such that

∥hc−φc,h∥1<2−h. \|h_c-\varphi_{c,h}\|_1<2^{-h}.

By §§2 and 4, for each fixed pair (c,h)(c,h) there is a measurable full-measure set Ec,hE_{c,h} on which

Vkφc,h(x)⟶p. V_k^{\varphi_{c,h}}(x)\longrightarrow p.

The index set ([1,2]∩Q)×N([1,2]\cap\mathbb Q)\times\mathbb N is countable, so

E=⋂c∈[1,2]∩Q⋂h=1∞Ec,h E=\bigcap_{c\in[1,2]\cap\mathbb Q}\bigcap_{h=1}^{\infty}E_{c,h}

is still measurable and has full measure. From now on, fix x∈Ex\in E. All rational scale ratios and all approximation accuracies are handled on the same set. No uncountable intersection over functions or ratios is taken.

6.2 The exact endpoint identity for interval weights

Set Nk=⌊c2k⌋N_k=\lfloor c2^k\rfloor. Since hc=c−11(0,c]h_c=c^{-1}\mathbf1_{(0,c]}, the sum includes exactly the integers 1≤n≤Nk1\le n\le N_k. Thus

2−k∑n∈Zhc(n/2k)Fn(x)=1c2k∑n=1NkFn(x)=Nkc2kANk(x). 2^{-k}\sum_{n\in\mathbb Z}h_c(n/2^k)F_n(x) =\frac1{c2^k}\sum_{n=1}^{N_k}F_n(x) =\frac{N_k}{c2^k}A_{N_k}(x).

Since ∣ANk∣≤1|A_{N_k}|\le1 and 0≤c2k−Nk<10\le c2^k-N_k<1, the left side differs from ANkA_{N_k} by at most (c2k)−1(c2^k)^{-1} in absolute value. For any fixed averaging weight φ\varphi, the triangle inequality now yields the paper's equation (3.16):

∣ANk(x)−Vkφ(x)∣≤1c2k+2−k∑n∈Z∣hc(n/2k)−φ(n/2k)∣.(R) |A_{N_k}(x)-V_k^\varphi(x)| \le\frac1{c2^k} +2^{-k}\sum_{n\in\mathbb Z}|h_c(n/2^k)-\varphi(n/2^k)|. \tag{R}

The function ∣hc−φ∣|h_c-\varphi| is bounded and compactly supported, and its only possible discontinuities are at 0,c0,c. It is therefore Riemann integrable, and the uniform-grid sum converges to ∥hc−φ∥1\|h_c-\varphi\|_1. Take φ=φc,h\varphi=\varphi_{c,h}, fix hh, and let k→∞k\to\infty. We obtain

lim sup⁡k→∞∣A⌊c2k⌋(x)−p∣≤2−h. \limsup_{k\to\infty}|A_{\lfloor c2^k\rfloor}(x)-p| \le 2^{-h}.

Now let h→∞h\to\infty. Then

A⌊c2k⌋(x)⟶pfor every c∈[1,2]∩Q,x∈E.(Q) A_{\lfloor c2^k\rfloor}(x)\longrightarrow p \quad\text{for every }c\in[1,2]\cap\mathbb Q, \quad x\in E. \tag{Q}

The weight is fixed before the scale tends to infinity. No uniform estimate is asserted for derivative constants, support radii, or oscillation constants that vary with the approximation accuracy.

6.3 Comparing two averaging lengths

Let (aj)(a_j) be a complex sequence with ∣aj∣≤1|a_j|\le1. For 1≤n≤N1\le n\le N,

1N∑j=1Naj−1n∑j=1naj=(1N−1n)∑j=1naj+1N∑j=n+1Naj. \begin{aligned} \frac1N\sum_{j=1}^{N}a_j-\frac1n\sum_{j=1}^{n}a_j &=\left(\frac1N-\frac1n\right)\sum_{j=1}^{n}a_j +\frac1N\sum_{j=n+1}^{N}a_j. \end{aligned}

Estimating the two terms separately yields

∣AN−An∣≤N−nN+N−nN=2(N−n)N.(L) |A_N-A_n|\le\frac{N-n}{N}+\frac{N-n}{N} =\frac{2(N-n)}{N}. \tag{L}

This inequality holds pointwise; it uses neither measure preservation nor mixing. It controls averages at the previously untreated lengths between neighboring grid points.

6.4 Fix the grid, take the scale limit, then refine the grid

Fix an integer s≥1s\ge1 and take the finite rational grid

ci=1+i/s,0≤i≤s. c_i=1+i/s, \quad 0\le i\le s.

For any N≥1N\ge1, choose the unique integer k≥0k\ge0 such that 2k≤N<2k+12^k\le N<2^{k+1}. Let ii be the largest index satisfying

n=⌊ci2k⌋≤N n=\lfloor c_i2^k\rfloor\le N

The index i=0i=0 always qualifies. The index i=si=s corresponds to 2k+1>N2^{k+1}>N, so i<si<s. By maximality and the distance between adjacent grid points,

0≤N−n≤2k/s+1. 0\le N-n\le 2^k/s+1.

By (L),

∣AN(x)−An(x)∣≤2s+21−k. |A_N(x)-A_n(x)| \le\frac{2}{s}+2^{1-k}.

By (Q), the averages at each fixed grid point converge to pp. Since the grid is finite, the maximum of their errors also tends to zero:

max⁡0≤i≤s∣A⌊ci2k⌋(x)−p∣⟶0. \max_{0\le i\le s} |A_{\lfloor c_i2^k\rfloor}(x)-p|\longrightarrow0.

Combining these estimates, we obtain

lim sup⁡N→∞∣AN(x)−p∣≤2/s. \limsup_{N\to\infty}|A_N(x)-p|\le2/s.

This inequality holds for every s≥1s\ge1, with the point still in the same set EE. Finally let s→∞s\to\infty. We conclude that AN(x)→pA_N(x)\to p through all positive integers.

Restore the original normalization of the functions and use S=TgS=T^g, bj=λj/gb_j=\lambda_j/g to obtain the conclusion in §1.1. Every exceptional set is measurable, and all unions and intersections are countable. This deduction therefore requires neither standardness nor completeness of the original probability space.

7. What has been established in this unit

Conditional on Proposition 3.5, the argument is complete in the following order:

  1. The uniform bound and oscillation estimate imply almost-everywhere convergence of the smooth averages for each fixed averaging weight.
  2. Ordinary mixing and the finite Hilbert-space inequality imply that the ordinary averages with distinct nonzero integer slopes converge in L2L^2 to the product of the integrals.
  3. Abel summation for positive and negative times shows that the same smooth averages converge in L2L^2 to that product. Fatou's lemma identifies the pointwise limit.
  4. Weights with the prescribed derivative bounds and vanishing moments approximate the interval weight in L1L^1.
  5. One countable intersection of full-measure sets covers the dyadic scales with all rational ratios. A finite grid and the length-comparison estimate recover all integers.

Proposition 3.5 itself and the local analytic estimates on which it depends have not been proved in this unit. The next task is to check the uniformity of C Theorem 2.2 in depth, number of blocks, and changes of input, and to inspect the exact results invoked from H and D.

The higher-order mixing assertion in R plays no part in this L2L^2 proof. It is a separate dependency of B and A. Combining the two arguments into the claim that “mixing makes everything independent” would misstate the proof.

8. Questions for further discussion

  • If the oscillation bound held only for one predetermined sequence of endpoints, would the recursive block selection in §2 still be possible?
  • If CC were allowed to depend on ww, where would the argument fail?
  • Why does the norm-convergence proof fix the correlation gap hh before sending the averaging length NN to infinity?
  • Which partial sums handle the negative-time support of the smooth weight in Abel summation?
  • Why does L1L^1 approximation of a positive interval weight not force the corrected signed weight to have a similar second moment?
  • Why is there no need in §6 to intersect the full-measure sets for all real cc?
  • If convergence were known only for N=2kN=2^k, why would the length-comparison estimate (L) not immediately send the remaining error to zero?

Guide to the original text

The fixed version of C is the principal source for this unit. Its page and result numbers are retained below:

  • p.3, first paragraph of §2.1: reduction by the greatest common divisor.
  • p.5, Definition 3.1, equations (3.1)–(3.2), and the next two paragraphs: averaging weights, the derivative class, and the smooth-function construction.
  • pp.8–9, Proposition 3.5, equations (3.9)–(3.11): smooth averages, their bound, and the oscillation estimate.
  • pp.9–10, Lemma 3.6: the proof from tail diameters to recursively chosen deterministic blocks.
  • p.10, Lemma 3.7: the finite Hilbert-space inequality.
  • pp.10–11, Lemma 3.8, equations (3.13)–(3.15): mixing, the L2L^2 induction, and smooth weights.
  • p.12, Lemma 3.9: convolution approximation and the Vandermonde moment correction.
  • pp.12–13, proof of the main theorem, equations (3.16)–(3.17): the countable full-measure intersection, interval-weight approximation, and the grid for all lengths.