Abstract
We prove a sharp (up to \(C_{\varepsilon }R^{\varepsilon }\)) \(L^{7}\) square function estimate for the moment curve in \(\mathbb{R}^{3}\).
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1 Introduction
We use a combination of high-low frequency analysis and induction to prove a sharp \(L^{7}\) square function estimate for the moment curve \(\mathcal {M}^{3}=\{(t,t^{2},t^{3}):0\le t\le 1\}\). As in [GWZ20] for the cone in \(\mathbb{R}^{3}\), this is an example of using techniques developed in decoupling theory [BD15] to prove square function estimates. It is worth noting that the only previous sharp square function estimates in restriction theory are for even \(L^{p}\) exponents, which often makes Fourier analysis problems more approachable.
In Fourier restriction theory, we are concerned with functions \(f=\sum _{\theta }f_{\theta}\) where \(\mathrm {supp}\widehat{f_{\theta}}\subset \theta \) and the \(\theta \) are pairwise disjoint. The shape of the Fourier support \(\cup \theta \) and the sets \(\theta \) determines the kinds of \(L^{p}\) bounds that \(f\) satisfies. By an \(L^{p}\) square function estimate, we mean an inequality of the form \(\|f\|_{L^{p}}\le C\|(\sum _{\theta }|f_{\theta}|^{2})^{1/2}\|_{L^{p}}\), while an \((\ell ^{2},L^{p})\) decoupling inequality has the form \(\|f\|_{L^{p}}\le C(\sum _{\theta }\|f_{\theta}\|_{L^{p}}^{2})^{1/2}\). Taking the \(L^{p}\) norm of each summand \(f_{\theta}\) separately makes it natural to approach decoupling using rescaling and induction-on-scales arguments, which Bourgain and Demeter did in [BD15]. Indeed, organize the \(\theta \) into larger (pairwise disjoint) sets \(\tau \) and suppose that for \(f_{\tau}:=\sum _{\theta \subset \tau}f_{\theta}\),
The desired decoupling inequality into the \(f_{\theta}\) then follows by rescaling each \(f_{\tau}\) and invoking induction to justify \(\|f_{\tau}\|_{L^{p}}\lessapprox (\sum _{\theta \subset \tau}\|f_{ \theta}\|_{L^{p}}^{2})^{1/2}\), since this inequality is equivalent to the initial problem but at a coarser scale. It is much less obvious how to use a multi-scale approach to prove square function estimates since we cannot rescale each \(f_{\tau}\) individually in the analogous intermediate expression \(\|(\sum _{\tau}|f_{\tau}|^{2})^{1/2}\|_{L^{p}}\). A major innovation of Guth-Wang-Zhang’s approach to the \(L^{4}\) square function estimate for the cone was to exploit Plancherel’s theorem and study \(\int (\sum _{\theta }|f_{\theta}|^{2})^{2}\) on the Fourier side. A detailed analysis of the Fourier support of \(\sum _{\theta }|f_{\theta}|^{2}\) then leads to an approximately equivalent expression for the \(L^{4}\) square function estimate called a wave envelope estimate. The advantage of the wave envelope expression is that it behaves well under rescaling and permits an induction-on-scales argument inspired by decoupling.
Guth-Wang-Zhang’s approach for the cone does not adapt to \(\mathcal {M}^{3}\). One immediate difference is that while it is possible to have a good understanding of the Fourier support of \(\sum _{\theta}|f_{\theta}|^{2}\), where \(\theta \) are pieces of a neighborhood of \(\mathcal {M}^{3}\), there is no Plancherel’s theorem for \(L^{7/2}\). This makes wave envelope expressions for \(\int (\sum _{\theta}|f_{\theta}|^{2})^{7/2}\) more complicated than in the \(p=4\) case, though it is still possible to identify a natural candidate. The main barrier to applying the Guth-Wang-Zhang inductive approach to \(\mathcal {M}^{3}\) is that there is no base case for the induction. The base case for the cone follows from approximating the cone by a cylindrical neighborhood of a parabola and invoking the classical Cordoba-Fefferman \(L^{4}\) square function estimate for the parabola [Có82]. There is no similar \(L^{7}\) estimate available for \(\mathcal {M}^{3}\) to establish a base case, so the inductive scheme breaks down.
Our argument builds on the high-low proof of decoupling for the moment curve, which is contained in [GM22b] and is based on the argument from [GMW20] for the parabola. The high-low method involves a stopping-time iteration depending on the behavior of square functions at many different scales. Nevertheless, it was not clear whether a high-low approach could be used to obtain the sharp \(L^{7}\) square function estimate for \(\mathcal {M}^{3}\). By introducing an algorithm inspired by wave envelope estimates, we are able to show that each case of the high-low iteration eventually leads to the desired \(L^{7}\) square function estimate or the initial problem at a coarser scale, which allows one to exploit induction. We provide an overview of the proof technique in §1.1.
For \(R\ge 1\), consider the anisotropic neighborhood
Partition this neighborhood of \(\mathcal {M}^{3}\) into canonical blocks \(\theta \), which have the form
For Schwartz functions \(f:\mathbb{R}^{3}\to \mathbb{C}\), define the Fourier projection onto \(\theta \) by \(f_{\theta}(x)=\int _{\theta }\widehat{f}(\xi )e^{2\pi i x\cdot \xi} d \xi \). Our main result is the following.
Theorem 1
For any \(\varepsilon >0\), there exists \(C_{\varepsilon }<\infty \) such that
for any Schwartz function \(f:\mathbb{R}^{3}\to \mathbb{C}\) with Fourier transform supported in \(\mathcal {M}^{3}(R)\).
We also obtain a version of Theorem 1 for curves in \(\mathbb{R}^{3}\) with torsion, which is explained in Appendix B. Theorem 1 is sharp, up to the \(C_{\varepsilon }R^{\varepsilon }\) factor. This may be seen from the constructive interference example which we now describe. Let \(\psi :\mathbb{R}^{3}\to [0,\infty )\) be a smooth bump function supported in the unit ball. For each \(\theta \), let \(\psi _{\theta}=|\theta |^{-1}\psi \circ T_{\theta}\) where \(T_{\theta}: \mathbb{R}^{3}\to \mathbb{R}^{3}\) is an affine transformation mapping an ellipsoid comparable to \(\theta \) to the unit ball. For a small universal constant \(c>0\), the support of \(\psi _{\theta}\) is completely contained in a canonical block at scale \(cR\), so Theorem 1 implies that
The function has amplitude \(\sim 1\) on the set \(\theta ^{*}=\{x\in \mathbb{R}^{3}:|x\cdot \xi |\le 1\quad \forall \xi \in \theta -\theta \}\) and decays rapidly away from \(\theta ^{*}\). The union of the sets \(\theta ^{*}\) is a bush centered at the origin of \(\sim R^{1/3}\times R^{2/3}\times R\) planks which are tangent to the light cone. A calculation shows that the right hand side of (3) is dominated by the portion of the bush at a distance \(\sim R\) from the origin, where the \(\theta ^{*}\) do not overlap, so
Finally, it is easy to see that in a neighborhood of radius \(\sim 1\) at the origin, , so the left hand side of (3) is bounded below by \(R^{7/3}\). This example also shows that no estimate of the form (2) holds in \(L^{p}\) if \(p>7\).
Estimates of the form (2) have a long history in harmonic analysis. The classical \(L^{4}\) square function estimate for the parabola is based on geometric observations by Fefferman [Fef73] and is recorded in [Có82]. The square function conjecture for paraboloids in \(\mathbb{R}^{n}\) (Conjecture 5.19 of [Dem20]) is known to imply sharp results for the Kakeya maximal function, the Bochner-Riesz means, and the Fourier restriction operator; see [Car15] and the references therein. In future work, we intend to explore analogous applications for the moment curve. Although square function estimates are known to have many applications, there are few sharp results of the form (2) in the literature. There has, however, been some partial progress on establishing square function estimates for the moment curve. In an unpublished work that was shared with the author, H. Jung proved a non-sharp version of Theorem 1 with a positive power of \(R\) in the upper bound. In [GGP21], the authors used approximate solution counting for Vinogradov systems to obtain square function estimates for the moment curve in \(\mathbb{R}^{n}\), but for non-sharp exponents \(2\le p\le 2n\) which are even. The only other sharp square function estimate we are aware of is for the cone in \(\mathbb{R}^{3}\) [GWZ20], which, by the work of [MSS92], resolves the local smoothing conjecture for the wave equation in \(\mathbb{R}^{2+1}\). Our proof of Theorem 1 uses both the square function estimate for the parabola in \(\mathbb{R}^{2}\) and for the cone in \(\mathbb{R}^{3}\).
The organization of this paper is as follows. In §1.1, we describe the main ideas behind the proof of Theorem 1. The proof of Theorem 1 happens in two steps. First, we prove a version of (2) where the terms in the square function are convolved with certain weights. Then we show that this averaged version implies Theorem 1. We introduce the square function constants \(\text{S}_{1}(R)\) and \(\text{S}_{2}(R)\) corresponding to these two versions of (2) in §1.2. We set up tools for the high-low argument in §2 and discuss the relevant geometry related to the moment curve and to the cone in §3. We devote §4 to a key technical step which unwinds the pruning process (see §1.1). The high-low method then allows us to bound the broad part of the left hand side of (2), when the integrand is dominated by a trilinear version of itself, which we carry out in §5. Finally we prove Theorem 1 by bounding \(\text{S}_{1}(R)\) and then \(\text{S}_{2}(R)\) in §6. Appendix A contains proofs of auxiliary square function and wave envelope estimates we require for the parabola and the cone. In Appendix B, we explain how to adapt the argument to obtain Theorem 1 for general curves \(\gamma (t)\) with torsion.
1.1 Overview of the proof of Theorem 1
In this section, we fix \(\varepsilon >0\) and a Schwartz function \(f:\mathbb{R}^{3}\to \mathbb{C}\). Let \(\theta \) denote canonical \(R^{-1/3}\times R^{-2/3}\times R^{-1}\) moment curve blocks. By pigeonholing arguments, it suffices to assume that either \(\|f_{\theta}\|_{\infty}\sim 1\) or \(\|f_{\theta}\|_{\infty}=0\) for each \(\theta \), and that for some \(\alpha >0\) and \(\beta >0\),
where \(U_{\alpha ,\beta }=\{x\in \mathbb{R}^{3}:|f(x)|>\alpha ,\quad \frac{\beta }{2}\le \sum _{ \theta}|f_{\theta}(x)|^{2}\le \beta \}\). Our goal is to show that
The initial step in bounding \(|U_{\alpha ,\beta }|\) involves the \(L^{6}\) trilinear restriction theorem for \(\mathcal {M}^{3}\). Since this theorem bounds trilinear expressions, we are actually bounding the broad part of \(U_{\alpha ,\beta }\) (which is the subset where \(|f|\lesssim |f_{1}f_{2}f_{3}|^{1/3}\) for Fourier projections \(f_{i}\) of \(f\) onto separated neighborhoods of \(\mathcal {M}^{3}\)). The narrow (or not broad) part of \(U_{\alpha ,\beta }\) is dealt with using a standard inductive argument.
The high-low method partitions \(U_{\alpha ,\beta }\) into \(\le \varepsilon ^{-1}\) many subsets \(\Omega _{k}\) which we bound in separate cases. Let \(R_{N-1}=R^{1-\varepsilon }\), let \(\tau _{N-1}\) denote \(R_{N-1}^{-1/3}\times R_{N-1}^{-2/3}\times R_{N-1}\) moment curve blocks, and let \(g_{N-1}=\sum _{\tau _{N-1}}|f_{\tau _{N-1}}|^{2}\). The high-low decomposition for \(g_{N-1}\) is \(g_{N-1}=g_{N-1}^{\ell}+g_{N-1}^{h}\) where for a bump function \(\eta _{N}\) equal to 1 on \(B_{R^{-1/3}}(0)\) and supported in \(B_{2R^{-1/3}}(0)\). A simple local \(L^{2}\)-orthogonality argument shows that \(|g_{N-1}^{\ell}|\lesssim \sum _{\theta}|f_{\theta}|^{2}\). Then since \(\sum _{\theta}|f_{\theta}|^{2}\sim \beta \) on \(U_{\alpha ,\beta }\), the assumption that \(A\beta \le g_{N-1}(x)\) implies that \(g_{N-1}(x)\le 2|g_{N-1}^{h}(x)|\), if \(A\ge 1\) is a sufficiently large constant. This leads to the first subset we bound:
which we will now describe how to control.
Applying the \(L^{6}\) multilinear restriction essentially yields
where \(R_{N-1}^{1/3}-\Omega _{N-1}\) means the \(R_{N-1}^{1/3}\)-neighborhood of \(\Omega _{N-1}\). Since the Fourier support of \(g_{N-1}\) is contained in \(\cup _{\tau _{N-1}}(\tau _{N-1}-\tau _{N-1})\subset B_{2R_{N-1}^{-1/3}}(0)\), \(g_{N-1}\) has roughly constant modulus on \({R_{N-1}^{1/3}}\)-balls on the spatial side. Therefore, since \(A\beta \le g_{N-1}\lesssim |g_{N-1}^{h}|\) on \(\Omega _{N-1}\),
Note that we chose to go from an \(L^{3}\) expression of \(g_{N-1}\) to an \(L^{4}\) expression. We did this because the Fourier support of \(g_{N-1}^{h}\) is contained in a neighborhood of the truncated cone, so we would like to use the sharp \(L^{4}\) square function estimate for the cone [GWZ20]. This allows us to control the integral on the right hand side above by
Since and there are \(\lesssim R^{\varepsilon /3}\) many \(\theta \) contained in each \(\tau _{N-1}\), the integral on the right hand side is bounded using Cauchy-Schwarz and Young’s convolution inequality by a constant factor times
The summary of the argument so far is that
Comparing with (4), we see that it suffices to check that \(\alpha \lesssim \beta \) and \(\int _{\mathbb{R}^{3}}|\sum _{\theta}|f_{\theta}|^{4}|^{2}\lesssim \int _{ \mathbb{R}^{3}}|\sum _{\theta}|f_{\theta}|^{2}|^{7/2}\). The first inequality is justified since morally, each \(|f_{\theta}|\) may be thought of as a sum amplitude 1 wave packets localized to non-overlapping translates of dual planks \(\theta ^{*}\), so \(|f_{\theta}|\lesssim |f_{\theta}|^{2}\). Then for \(x\in U_{\alpha ,\beta }\), we have \(\alpha \lesssim |\sum _{\theta }f_{\theta}(x)|\lesssim \sum _{\theta}|f_{ \theta}(x)|\lesssim \sum _{\theta}|f_{\theta}(x)|^{2}\lesssim \beta \). The second inequality is justified by the assumption that \(\|f_{\theta}\|_{\infty}\lesssim 1\), so \(\sum _{\theta}|f_{\theta}|^{4}\lesssim \sum _{\theta}|f_{\theta}|^{7/2}\), and then using \(\|\cdot \|_{\ell ^{7/2}}\le \|\cdot \|_{\ell ^{2}}\). This concludes the bound of \(|\Omega _{N-1}|\), which only involved a local multilinear restriction estimate, high-frequency dominance with the locally constant property, and applying the \(L^{4}\) square function estimate for the cone. For the remaining parts of \(U_{\alpha ,\beta }\), we will see that an additional idea is required.
Intermediate scales: Let \(R_{k}=R^{k\varepsilon }\), let \(\tau _{k}\) be canonical \(R_{k}^{-1/3}\times R_{k}^{-2/3}\times R_{k}^{-1}\) moment curve blocks, and let \(g_{k}=\sum _{\tau _{k}}|f_{\tau _{k}}|^{2}\). Decompose \(g_{k}\) into high-low parts \(g_{k}=g_{k}^{\ell}+g_{k}^{h}\) by defining , where \(\eta _{k}\) is a bump function equal to 1 on \(B_{R_{k+1}^{-1/3}}(0)\). The \((N-k)\)th subset of \(U_{\alpha ,\beta }\) that we consider is
As in the analysis of \(\Omega _{N-1}\), we can show that on \(\Omega _{k}\), \(g_{k}\) is high-dominated. After applying the \(L^{6}\) trilinear restriction and using that \(A^{N-k}\beta \le g_{k}\lesssim |g_{k}^{h}|\) on \(\Omega _{k}\), we have
Again, \(g_{k}^{h}\) is Fourier supported on the \(R_{k}^{-1/3}\)-dilation of the truncated cone, so we may apply the \(L^{4}\) square function estimate for the cone, yielding
Here, unlike in the analysis of \(\Omega _{N-1}\), \(\tau _{k}\) may be much coarser than \(\theta \), so we cannot use trivial inequalities and the assumption that \(\|f_{\theta}\|_{L^{\infty}}\lesssim 1\) to arrive at the right hand side of (4). To provide an alternative \(L^{\infty}\) bound for each \(f_{\tau _{k}}\), we perform a pruning process on the wave packets. This pruning process is the same as the one from [GMW20], in which we argue that on \(\Omega _{k}\subset U_{\alpha ,\beta }\), \(f\) may be replaced by a version \(f^{k}=\sum _{\tau _{k}} f_{\tau _{k}}^{k}\) where each \(f_{\tau _{k}}^{k}\) only has wave packets with amplitude \(\lesssim \beta /\alpha \). The pruned \(f_{\tau _{k}}^{k}\) satisfy the property that \(\|f_{\tau _{k}}^{k}\|_{\infty}\lesssim \frac{\beta }{\alpha }\). Using \(f^{k}\) in place of \(f\) in (5) and the good \(L^{\infty}\) bound for each \(f_{\tau _{k}}^{k}\), we arrive at the inequality
which, using \(\|\cdot \|_{\ell ^{7/2}}\le \|\cdot \|_{\ell ^{2}}\), implies that
The left hand side looks good because it is an \(L^{7}\) expression. It remains to consider how to bound the right hand side by the \(L^{7}\) integral of the square function at our desired scale \(\theta \). It looks as though the right hand side is partial progress towards \(\sum _{\theta}|f_{\theta}|^{2}\), so we would like to invoke induction to finish the argument. Indeed, if our goal were to prove an \((\ell ^{2},L^{7})\) decoupling estimate and we had shown
then we could rescale each \(f_{\tau _{k}}\) and invoke induction on scales to justify \(\|f_{\tau _{k}}\|_{L^{7}(\mathbb{R}^{3})}\lesssim (\sum _{\theta \subset \tau _{k}}\|f_{\theta}\|_{L^{7}(\mathbb{R}^{3})}^{2})^{1/2}\), which combines with the displayed inequality to give the desired \((\ell ^{2},L^{7})\) estimate. The main difficulty of proving a square function estimate compared to a decoupling estimate is that the integrand on the right hand side of (6) involves all of the \(f_{\tau _{k}}^{k}\), so we cannot rescale each \(f_{\tau _{k}}^{k}\) individually and invoke induction.
To address this problem, we introduce an algorithm which either isolates the different \(f_{\tau _{k}}^{k}\) to permit rescaling and induction, or allows us to further refine \(\sum _{\tau _{k}}|f_{\tau _{k}}^{k}|^{2}\) pointwise to \(\sum _{\tau '}|f_{\tau '}|^{2}\), where the \(\tau '\) are closer to our goal \(\theta \) than the \(\tau _{k}\). Our algorithm begins by using the wave envelope estimate Theorem 1.3 from [GWZ20] in place of the \(L^{4}\) square function estimate to bound \(g_{k}^{h}\). The wave envelope estimate for the cone replaces the standard square function integral by a controlled number of more-refined expressions. To simplify the explanation of our strategy, we will consider the special case coming from the wave envelope estimate in which \(\int |\sum _{\tau _{k}}|f_{\tau _{k}}^{k}|^{4}|^{2}\) from (5) is dominated by the part of the domain on which only one summand \(|f_{\tau _{k}}^{k}|\) is large at a time. Otherwise repeating the reasoning that led to (6), this yields
At first sight, the integral on the right hand side of (7) looks similar to
Since each \(f_{\tau _{k}}\) is integrated individually, this expression can be handled by induction as follows. Let \(\text{S}(R)\) be the smallest constant for which
for any \(f\) satisfying the hypotheses of Theorem 1. Using affine rescaling of the moment curve, (8) is bounded by
Supposing that \(R_{k}>R^{C_{0}\varepsilon }\), this would be a favorable scenario since the multi-scale inequality \(S(R)\lesssim _{\varepsilon }R^{C\varepsilon } S(R/R_{k})\) implies that \(S(R)\lesssim _{\delta }R^{\delta }\) for any \(\delta >0\). The issue with this argument is that the \(f_{\tau _{k}}^{k}\) in (7) are different from the \(f_{\tau _{k}}\) in (8). The pruning process which leads to the favorable \(L^{\infty}\) bounds for \(f_{\tau _{k}}^{k}\) also changes the Fourier support from \(\cup _{\theta \subset \tau _{k}}\theta \) to potentially all of \(\tau _{k}\). A rescaling argument may still be used to argue that
but then we need to analyze the expression on the right hand side. The bulk of the new technical work in this paper is to perform a delicate algorithm addressing all of the cases from the wave envelope estimate (which is applied repeatedly) while “unpruning” \(f^{k}\) (going from expressions with \(f^{k}\) to \(f^{k+1}\) and eventually to \(f^{N}=f\)) and carefully keeping track of constants to ensure the induction closes. Eventually, we bound the right hand side of (7) by an expression like
where \(\delta >0\) may be arbitrarily small. This is again a favorable case since \(S(R)\le C_{\delta ,\varepsilon } R^{\delta +\varepsilon } S(R^{\varepsilon })^{\varepsilon ^{-1}-C_{0}}\) for any \(\delta >0\) and any \(\varepsilon >0\) implies the desired bound for \(S(R)\).
Small scale: \(R_{k}\le R^{C_{0}\varepsilon }\). In this case, the remaining subset of \(U_{\alpha ,\beta }\) is
The argument for the intermediate scales case no longer works when \(R_{k}\) is too small since we could conclude, for example, that \(S(R)\le C_{\delta ,\varepsilon }R^{\delta }S(R^{\varepsilon })^{\varepsilon ^{-1}}\). This would not lead to the desired bound \(S(R)\lesssim _{\delta }R^{\delta }\). Instead, we use trivial bounds based on the definition of \(L\). For each \(x\in L\), for any \(l=C_{0},\ldots ,N-1\), we may write
Then using \(l=C_{0}\),
which gives the bound \(S(R)\lesssim R^{C_{0}\varepsilon }\) directly.
The conclusion of the high-low argument from each of the previous cases is that for any \(\delta ,\varepsilon >0\) and \(C_{0}>0\),
The exact version of the multi-scale inequality we prove is in Lemma 6.7. We show in §6.2 how the multi-scale inequality implies the desired bound for \(S(R)\).
1.2 Definitions of the square function constants \(S_{1}(R)\) and \(S_{2}(R)\)
Technically, the result of our high-low argument is
for appropriate \(L^{1}\)-normalized weight functions \(\omega _{\theta}\) adapted to \(\theta ^{*}\). While the locally constant property (see Lemma 2.2) tells us that pointwise,
it is not generally true that the reverse inequality holds, either pointwise or in \(L^{7/2}\). Indeed, let \({\mathbf{{v}}}_{\theta}\in \mathbb{R}^{3}\) be a unit vector in the direction of the \(R\)-long side of \(\theta ^{*}\), let \(T_{\theta}\) be an \(R^{2/3}\times R^{2/3}\times R\) tube centered at the origin with orientation \({\mathbf{{v}}}_{\theta}\), and let each \(|f_{\theta}|^{2}(x)\approx \chi _{T_{\theta}}(x-R{\mathbf{{v}}}_{\theta})\). Then
since the \(|f_{\theta}|^{2}\) are essentially disjointly supported. On the other hand, after averaging, \(\sum _{\theta}|f_{\theta}|^{2}*\omega _{\theta}\gtrsim R^{1/3}\) on a ball of radius \(\sim R^{2/3}\) centered at the origin, giving the lower bound
Therefore, the version of a square function estimate (9) that we obtain from the high-low argument is ostensibly weaker than our goal. After proving (9), we use an inductive argument to upgrade it to (2).
Definition 1
Let \(R\ge 10\). Let \(S_{1}(R)\) be the infimum of \(A>0\) such that
for any Schwartz function \(f:\mathbb{R}^{3}\to \mathbb{C}\) with Fourier transform supported in \(\mathcal {M}^{3}(R)\).
Definition 2
Let \(R\ge 10\). Let \(S_{2}(R)\) be the infimum of \(B>0\) such that
for any Schwartz function \(f:\mathbb{R}^{3}\to \mathbb{C}\) with Fourier transform supported in \(\mathcal {M}^{3}(R)\).
2 Set-up for the high-low analysis
In this section, we set-up the notation and basic properties of the high-low analysis of square functions at various scales. This is analogous to the high-low set-up from [GMW20].
Begin with precise definitions of canonical blocks of the moment curve.
Definition 3
Canonical moment curve blocks
For \(S\in 2^{\mathbb{N}}\), consider the anisotropic neighborhood
Define \({\mathbf{{S}}}(S^{-1})\) to be the following collection of canonical moment curve blocks at scale \(S\) which partition \(\mathcal {M}^{3}(S^{3})\):
The (not unit-normalized) Frenet frame for the moment curve \(\mathcal {M}^{3}\) at \(t\in [0,1]\) is
If \(\tau \in{\mathbf{{S}}}(S^{-1})\) is the \(\ell \)th moment curve block
then \(\tau \) is comparable to the set
By comparable, we mean that there is an absolute constant \(C>0\) for which \(C^{-1}\tau \) is contained in the displayed set and \(C\tau \) contains the displayed set, where the dilations are taken with respect to the centroid of \(\tau \). Define the dual set \(\tau ^{*}\) by
We sometimes refer to the set \(\tau ^{*}\) as well as its translates as wave packets.
Next, we fix some notation for the scales. Let \(\varepsilon >0\). To prove Theorem 1, it suffices to assume that \(R\) is larger than a constant which depends on \(\varepsilon \). Consider scales \(R_{k}\in 8^{\mathbb{N}}\) closest to \(R^{k\varepsilon }\), for \(k=1,\ldots ,N\) and \(R_{N}\le R\le R^{\varepsilon }R_{N}\). Since \(R\) differs from \(R_{N}\) at most by a factor of \(R^{\varepsilon }\), we will assume that \(R=R_{N}\). The relationship between the parameters is
Fix notation for moment curve blocks of various sizes.
-
(1)
Let \(\theta \) denote \(\sim R^{-\frac{1}{3}}\times R^{-\frac{2}{3}}\times R^{-1}\) moment curve blocks from the collection \({\mathbf{{S}}}(R^{-1/3})\).
-
(2)
Let \(\tau _{k}\) denote \(\sim R_{k}^{-\frac{1}{3}}\times R_{k}^{-\frac{2}{3}}\times R_{k}^{-1}\) moment curve blocks from the collection \({\mathbf{{S}}}(R_{k}^{-1/3})\).
The definitions of \(\theta ,\tau _{k}\) provide the additional property that if \(k< m\) and \(\tau _{k}\cap \tau _{m}\neq\emptyset \), then \(\tau _{m}\subset \tau _{k}\).
Fix a ball \(B_{R}\subset \mathbb{R}^{3}\) of radius \(R\) as well as a Schwartz function \(f:\mathbb{R}^{3}\to \mathbb{C}\) with Fourier transform supported in \(\mathcal {M}^{3}(R)\). The parameters \(\alpha ,\beta >0\) describe the set
The weight function \(\omega _{\theta}\) is defined in Definition 5 below. We assume throughout this section (and until §6.1) that the \(f_{\theta}\) satisfy the extra condition that
2.1 A pruning step
We define wave packets associated to \(f_{\tau _{k}}\) and sort them according to an amplitude condition which depends on the parameters \(\alpha \) and \(\beta \).
For each \(\tau _{k}\), let \(\mathbb{T}_{\tau _{k}}\) contain \(\tau _{k}^{*}\) and its translates \(T_{\tau _{k}}\) which tile \(\mathbb{R}^{3}\). Fix an auxiliary function \(\varphi (\xi )\) which is a bump function supported in \([-\frac{1}{4},\frac{1}{4}]^{3}\). For each \(m\in \mathbb{Z}^{3}\), let
where \(c\) is chosen so that . Since is a rapidly decaying function, for any \(n\in \mathbb{N}\), there exists \(C_{n}>0\) such that
Define the partition of unity \(\psi _{T_{\tau _{k}}}\) associated to \({\tau _{k}}\) to be \(\psi _{T_{\tau _{k}}}(x)=\psi _{m}\circ A_{\tau _{k}}\), where \(A_{\tau _{k}}\) is a linear transformations taking \(\tau _{k}^{*}\) to \([-\frac{1}{2},\frac{1}{2}]^{3}\) and \(A_{\tau _{k}}(T_{\tau _{k}})=m+[-\frac{1}{2},\frac{1}{2}]^{3}\). The important properties of \(\psi _{T_{\tau _{k}}}\) are (1) rapid decay off of \(T_{\tau _{k}}\) and (2) Fourier support contained in \(\tau _{k}\) translated to the origin. We sort the wave packets \(\mathbb{T}_{\tau _{k}}=\mathbb{T}_{\tau _{k}}^{g}\sqcup \mathbb{T}_{\tau _{k}}^{b}\) into “good” and “bad” sets, and define corresponding versions of \(f\), as follows.
Remark 1
In the following definitions, let \(K\ge 1\) be a large parameter which will be used to define the broad set in Proposition 5.1. Also, \(A=A(\varepsilon )\gg 1\) is a large enough constant (determined by Lemma 2.6) which also satisfies \(A\ge D\), where \(D\) is from Lemma 2.4.
Definition 4
Pruning with respect to \(\tau _{k}\)
Let \(f^{N}=f\), \(f^{N}_{\tau _{N}}=f_{\theta}\). For each \(1\le k\le N-1\), let
For each \(k\), the \(k\)th version of \(f\) is \(f^{k}=\underset{\tau _{k}}{\sum} f_{\tau _{k}}^{k}\).
Remark 2
We may assume that \(\alpha \lesssim R^{C_{0}}\beta \). This will be discussed in Proposition 6.4and Corollary 6.5, which involve pigeonholing the wave packets of \(f\).
In the following lemma, we assume that the \(f_{\theta}\) satisfy (12) and \(f=\sum _{\theta }f_{\theta}\) has been pruned according to the above definition.
Lemma 2.1
Properties of \(f^{k}\)
-
(1)
\(| f_{\tau _{k}}^{k} (x) | \le |f_{ \tau _{k}}^{k+1}(x)|\lesssim \# \theta \subset \tau _{k}\).
-
(2)
\(\| f_{\tau _{k}}^{k} \|_{L^{\infty}(\mathbb{R}^{3})} \le K^{3}A^{N-k+1} \frac{\beta }{\alpha }\).
-
(3)
For \(R\) sufficiently large depending on \(\varepsilon \), \(\textit{supp} \widehat{f_{\tau _{k}}^{k}}\subset 3\tau _{k} \).
Proof
For the first property, recall that \(\sum _{T_{\tau _{k}} \in \mathbb{T}_{\tau _{k}}}\psi _{T_{\tau _{k}}}\) is a partition of unity so we may iterate the inequalities
The first property follows from our assumption (12) that each \(\|f_{\theta}\|_{L^{\infty}(\mathbb{R}^{3})}\lesssim 1\). For the \(L^{\infty}\) bound in the second property, write
By the definition of \(\mathbb{T}_{\tau _{k}}^{g}\), \(\|\psi _{T_{\tau _{k}}}^{1/2}f_{\tau _{k}}^{k+1}\|_{\infty}\le K^{3} A^{N-k+1} \frac{\beta }{\alpha }\).
The third property depends on the Fourier support of \(\psi _{T_{\tau _{k}}}\), which is contained in \(\tau _{k}\) shifted to the origin. Note if each \(f_{\tau _{k}}^{k+1}\) has Fourier support in \(\cup _{\tau _{k+1}\subset \tau _{k}}3\tau _{k+1}\), then \(\mathrm {supp}\widehat{f_{\gamma _{k}}^{k}}\) is contained in \(3\tau _{k}\). □
Definition 5
Let \(\phi :\mathbb{R}^{3}\to \mathbb{R}\) be a smooth, radial function supported in \([-\frac{1}{4},\frac{1}{4}]^{3}\) and satisfying when \(|x|\le 1\). Then define \(w:\mathbb{R}^{3}\to [0,\infty )\) by
Let \(B\subset \mathbb{R}^{3}\) denote the unit ball centered at the origin. For any set \(U=T(B)\) where \(T\) is an affine transformation \(T:\mathbb{R}^{3}\to \mathbb{R}^{3}\), define
For each \(\tau _{k}\), let \(A_{\tau _{k}}\) be a linear transformation mapping \(\tau _{k}^{*}\) to the unit cube and define \(\omega _{\tau _{k}}\) by
Let the capital-W version of weight functions denote the \(L^{\infty}\)-normalized (as opposed to \(L^{1}\)-normalized) versions, so for example, for any ball \(B_{s}\), \(W_{B_{s}}(x)=|B_{s}|w_{B_{s}}(x)\). If a weight function has subscript which is only a scale, say \(s\), then the functions \(w_{s},W_{s}\) are weight functions localized to the \(s\)-ball centered at the origin.
Remark 3
Note the additional property that \(\widehat{w}\) is supported in \([-\frac{1}{2},\frac{1}{2}]^{3}\), so each \(w_{B_{s}}\) is Fourier supported in an \(s^{-1}\)-neighborhood of the origin. Finally, note the property that if \(A_{1},A_{2}\) are affine transformations of the unit ball and \(A_{1}\subset A_{2}\), then \(w_{A_{1}}*w_{A_{2}}\lesssim w_{A_{2}}\).
Next, we record the locally constant property. By locally constant property, we mean that if a function \(f\) has Fourier transform supported in a convex set \(A\), then \(|f|\) is bounded above by an averaged version of \(|f|\) over a dual set \(A^{*}\).
Lemma 2.2
Locally constant property
For each \(\tau _{k}\) and \(T_{\tau _{k}}\in \mathbb{T}_{\tau _{k}}\),
Also, for any \(R_{k}^{1/3}\)-ball \(B_{R_{k}^{1/3}}\),
Because the pruned versions of \(f\) and \(f_{\tau _{k}}\) have essentially the same Fourier supports as the unpruned versions, the locally constant lemma applies to the pruned versions as well.
Proof of Lemma 2.2
For the first claim, we write the argument for \(f_{\tau _{k}}\) in detail. Let \(\rho _{\tau _{k}}\) be a bump function equal to 1 on \(\tau _{k}\) and supported in \(2\tau _{k}\). Then using Fourier inversion and Hölder’s inequality,
Since \(\rho _{\tau _{k}}\) may be taken to be an affine transformation of a standard bump function adapted to the unit ball, is a constant. The function decays rapidly off of \(\tau _{k}^{*}\), so . Since for any \(T_{\tau _{k}}\in \mathbb{T}_{\tau _{k}}\), \(\omega _{\tau _{k}}(y)\sim \omega _{\tau _{k}}(y')\) for all \(y,y'\in T_{\tau _{k}}\), we have
For the second part of the lemma, repeat analogous steps as above, except begin with \(\rho _{\tau _{k}}\) which is identically 1 on a ball of radius \(2R_{k}^{-1/3}\) containing \(\tau _{k}\). Then
where we used that each \(\rho _{\tau _{k}}\) is a translate of a single function \(\rho _{R^{-1/3}}\). The rest of the argument is analogous to the first part. □
The following local \(L^{2}\)-orthogonality lemma which is Lemma 3 in [GM22b].
Lemma 2.3
Local \(L^{2}\) orthogonality
Let \(U=T(B)\) where \(B\) is the unit ball centered at the origin and \(T:\mathbb{R}^{3}\to \mathbb{R}^{3}\) is an affine transformation. Let \(h:\mathbb{R}^{3}\to \mathbb{C}\) be a Schwartz function with Fourier transform supported in a disjoint union \(X=\sqcup _{k} X_{k}\), where \(X_{k}\subset B\) are Lebesgue measurable. If the maximum overlap of the sets \(X_{k}+U^{*}\) is \(L\), then
where \(h_{X_{k}}=\int _{X_{k}}\widehat{h}(\xi )e^{2\pi i x\cdot \xi}d\xi \).
Here, we may take \(\{x:|x\cdot \xi |\le 1\quad \forall \xi \in U-U\}\) as the definition of \(U^{*}\). We will include a sketch of the proof for future reference.
Proof
By Plancherel’s theorem, we have
Since \(\widehat{h_{X}}=\sum _{k}\widehat{h_{X_{k}}}\), \(\int \widehat{h_{X}}\overline{\widehat{h_{X}}*\widehat{w_{U}}}=\sum _{X_{k}} \sum _{X_{k}'}\int \widehat{h_{X_{k}}} \overline{\widehat{h_{X_{k}'}}*\widehat{w_{U}}}\). For each \(X_{k}\), the integral on the right hand side vanishes except for \(\lesssim L\) many choices of \(X_{k}'\). □
2.2 High-low frequency decomposition of square functions
Definition 6
Auxiliary functions
Let \(\eta :\mathbb{R}^{3}\to [0,\infty )\) be a radial, smooth bump function satisfying \(\eta (x)=1\) on \(B_{1/2}\) and \(\mathrm {supp}\eta \subset B_{1}\). Then for each \(s>0\), let
We will sometimes abuse notation by denoting , where \(h\) is some Schwartz function. Also define \(\eta _{s}(x)=\eta _{\le s}-\eta _{\le s/2}\).
Fix \(N_{0}< N-1\) which will be specified in §6.2.
Definition 7
For \(N_{0}\le k\le N-1\), let
In the following definition, \(A\gg 1\) is the same constant that goes into the pruning definition of \(f^{k}\).
Definition 8
Define the high set by
For each \(k=N_{0},\ldots ,N-2\), let \(H=\Omega _{N-1}\) and let
Define the low set to be
Lemma 2.4
Low lemma
There is an absolute constant \(D>0\) so that for each \(x\), \(|g_{k}^{\ell}(x)|\le D g_{k+1}(x)\).
Proof
We perform a pointwise version of the argument in the proof of local/global \(L^{2}\)-orthogonality (Lemma 2.3). For each \(f_{\tau _{k}}^{k+1}\), by Plancherel’s theorem,
The integrand is supported in \((2\tau _{k+1}-2\tau _{k+1}')\cap B_{R_{k+1}^{-1/3}}\). This means that the integral vanishes unless \(\tau _{k+1}\) is within \(\sim R_{k+1}^{-1/3}\) of \(\tau _{k+1}'\), in which case we write \(\tau _{k+1}\sim \tau _{k+1}'\). Then
Use Plancherel’s theorem again to get back to a convolution in \(x\) and conclude that
By the locally constant property (Lemma 2.2) and (1) of Lemma 2.1,
It remains to note that
since \(\tau _{k}^{*}\subset \tau _{k+1}^{*}\) and is an \(L^{1}\)-normalized function that is rapidly decaying away from \(B_{R_{k+1}^{1/3}}(0)\). □
Corollary 2.5
High-dominance on \(\Omega _{k}\)
For \(R\) large enough depending on \(\varepsilon \), \(g_{k}(x)\le 2|g_{k}^{h}(x)|\) for all \(x\in \Omega _{k}\).
Proof
This follows directly from Lemma 2.4. Indeed, since \(g_{k}(x)=g_{k}^{\ell}(x)+g_{k}^{h}(x)\), the inequality \(g_{k}(x)>2|g_{k}^{h}(x)|\) implies that \(g_{k}(x)<2|g_{k}^{\ell}(x)|\). Then by Lemma 2.4, \(|g_{k}(x)|<2D g_{k+1}(x)\). Since \(x\in \Omega _{k}\), \(g_{k+1}(x)\le A^{N-k-1}\beta \), which altogether gives the upper bound
The contradicts the property that on \(\Omega _{k}\), \(A^{N-k}\beta \le g_{k}(x)\), for \(A\) sufficiently larger than \(D\), which finishes the proof. □
Lemma 2.6
Pruning lemma
For any \(s\ge R^{-\varepsilon /3}\) and \(\tau \in{\mathbf{{S}}}(s)\),
Proof
Begin by proving the first claim about \(\Omega _{k}\). By the definition of the pruning process, we have
where formally, the subscript \(\tau \) means \(f_{\tau}=\sum _{\theta \subset \tau}f_{\theta}\) and \(f_{\tau}^{m}=\sum _{\tau _{m}\subset \tau}f_{\tau _{m}}^{m}\). We will show that each difference in the sum is much smaller than \(\alpha \). For each \(N-1\ge m\ge k+1\) and \(\tau _{m}\),
Let \(c_{\tilde{T}_{\tau _{m}}}\) denote the center of \(\tilde{T}_{\tau _{m}}\) and note the pointwise inequality
which means that
where we used the locally constant property in the second to last inequality. The last inequality is justified by the fact that \(\omega _{\tau _{m}}(x-c_{\tilde{T}_{\tau _{m}}})\sim \omega _{\tau _{m}}(x-y)\) for any \(y\in \tilde{T}_{\tau _{m}}\), and we have the pointwise relation \(\omega _{\tau _{m}}*\omega _{\tau _{m}}\lesssim \omega _{\tau _{m}}\). Then
At this point, choose \(A\) sufficiently large determined by the proof of Corollary 2.5 and so that if \(g_{m}(x)\le A^{N-m}\beta \), then the above inequality implies that
This finishes the proof since the number of terms in (13) is bounded by \(N\le \varepsilon ^{-1}\). The argument for the pruning on \(L\) is analogous. □
3 Geometry for the cone and the moment curve
We have seen in Corollary 2.5 that on \(\Omega _{k}\), \(g_{k}\) is high-dominated. We will now describe how to use the wave envelope estimate for the cone (Theorem 1.3 from [GWZ20]) to control the high part of \(g_{k}\).
Begin by describing the cone set-up using the rotated coordinate system from §5 of [GWZ20]. Define the truncated cone by \(\Gamma = \{r(1,\omega ,\frac{1}{2}\omega ^{2}):\frac{1}{2}\le r\le 1,\quad | \omega |\le 1\}\). We consider the neighborhood
where \(S\ge 1\) is dyadic. For \(|\omega |\le 1\), we will use the (not unit-normalized) frame
Define a cone plank \(\tau \) of dimension \(1\times S^{-1}\times S^{-2}\) and centered at \((1,\omega ,\frac{1}{2}\omega ^{2})\in \Gamma \) by
Let \({\mathbf{{S}}}_{S^{-1}}\) denote a collection of \(1\times S^{-1}\times S^{-2}\) conical blocks \(\tau \) which approximately partition \(\Gamma (S^{2})\). The definitions and notation we use are compatible with those in §3 of [GWZ20].
Recall that our goal in this section is to bound the high part of \(g_{k}\). The summands of \(g_{k}\) have Fourier support in \(2\tau _{k}-2\tau _{k}\), where \(\tau _{k}\in{\mathbf{{S}}}(R_{k}^{-1/3})\) (noting that \({\mathbf{{S}}}(R_{k}^{-1/3})\) refers to moment curve blocks defined at the beginning of §2). Removing the low part cuts away a ball of radius \(R_{k+1}^{-1/3}\). In Proposition 3.1, we will essentially show that \((2\tau _{k}-2\tau _{k})\setminus B_{R_{k+1}^{-1/3}}\) may be identified with a conical plank \(\tau \in{\mathbf{{S}}}_{R_{k}^{-1/3}}\).
Let \(S\ge 1\) be a dyadic parameter that will be chosen to be sufficiently large in Proposition 3.1. Suppose that \(\tau \in{\mathbf{{S}}}(S^{-1})\) is the \(l\)th piece, meaning that
where \(l\in \{0,\ldots ,S-1\}\). Using the Frenet frame description from (10), the set \((10\tau -10\tau )\setminus B_{(4S)^{-1}}(0)\) is contained in
Define the linear transformation \(T:\mathbb{R}^{3}\to \mathbb{R}^{3}\) by
Proposition 3.1
Let \(S\in 2^{\mathbb{N}}\) be larger than some absolute constant. After dilating by \(S\), the sets \(T[(10\tau -10\tau )\setminus B_{(4S)^{-1}}(0)]\) with \(\tau \in{\mathbf{{S}}}(S^{-1})\), are comparable to the cone planks from \({\mathbf{{S}}}_{S^{-1}}\).
Proof
The image of the set (15) under \(T\) is
Define \(\omega =lS^{-1}\). Since \(T({\mathbf{{T}}}(lS^{-1}))={\mathbf{{c}}}(lS^{-1})\) and \(T({\mathbf{{N}}}(lS^{-1}))\cdot{\mathbf{{t}}}(lS^{-1})=0\), it is easy to see that the set \(T(\tilde{\tau})\) is comparable to the \(S^{-1}\) dilation of (14). □
Next, we define moment curve wave envelopes, which are roughly the smallest convex sets containing wave packets from neighboring moment curve blocks.
Definition 9
Let \(1\le S^{3}\le R \). For \(\tau \in{\mathbf{{S}}}(S^{-1})\) which is the \(\ell \)th block, define the moment curve wave envelope \(V_{\tau ,R}\) to be
We will compare these with wave envelopes for the cone defined in §3 from [GWZ20]. Again let \(1\le S^{3}\le R\). Using our notation, if \(\tau '\in{\mathbf{{S}}}_{S^{-1}}\) is given by (14), then the cone wave envelope \(U_{\tau ',R^{2/3}}\) is defined by
After applying a linear transformation, the \(R^{-1/3}\)-dilation of the moment curve wave envelope \(V_{\tau ,R}\) is comparable to a cone wave envelope \(U_{\tau ',R^{2/3}}\).
Proposition 3.2
Let \(T\) be the linear transformation (16) and let \(S\) be a sufficiently large dyadic number with \(1\le S^{3}\le R\). Then for each \(\tau \in{\mathbf{{S}}}(S^{-1})\), there is a \(\tau '\in{\mathbf{{S}}}_{S^{-1}}\) for which \(R^{-1/3}\cdot [(T^{t})^{-1}V_{\tau ,R}]\) is comparable to \(U_{\tau ',R^{2/3}}\).
Proof
Note that \((T^{t})^{-1}(x,y,z)=(x,2y,6z)\). The \(R^{-1/3}\)-dilation of the image of the wave envelope \(V_{\tau ,R}\) under \((T^{t})^{-1}\) is
Applying a Gram-Schmidt process to the vectors, we see that the above set is comparable to
Define \(\omega =lS^{-1}\). Then it is clear that the above set is comparable to \(U_{\tau ',R^{2/3}}\) where \(\tau '\in{\mathbf{{S}}}_{S^{-1}}\) is centered at \((1,\omega ,\frac{1}{2}\omega ^{2})\), as require by the proposition. □
3.1 High-frequency analysis
Now that we have identified moment curve blocks with cone planks and moment curve wave envelopes with cone wave envelopes, we are prepared to use Theorem 1.3 from [GWZ20] to control the high part of square functions. Recall the theorem statement.
Theorem 3.3
Theorem 1.3 from [GWZ20]
For each \(\delta >0\), there exists \(B_{\delta }\in (0,\infty )\) so that
for any Schwartz function \(f:\mathbb{R}^{3}\to \mathbb{C}\) with Fourier transform supported in \(\Gamma (R)\).
The initial sum on the right hand side is over dyadic \(\sigma \), \(R^{-1/2}\le \sigma \le 1\). Whenever we sum over an interval \((a,b)\), we always mean the numbers in \(2^{\mathbb{Z}}\cap (a,b)\).
Lemma 3.4
High lemma
For each \(\delta >0\), there is \(B_{\delta }\in (0,\infty )\) so that the following holds. For any \(k\), there is some dyadic scale \(R_{k+1}^{-1/3}\le s\le 10 R_{k}^{-1/3}\) for which
Proof
First describe the Fourier support of \(g_{k}^{h}\). By (3) of Lemma 2.1, the support of \(\widehat{|f_{\tau _{k}}^{k+1}|^{2}}\) is \(2(\tau _{k}-\tau _{k})\). The high-frequency cutoff removes a ball of radius \(R_{k+1}^{-1/3}\), so \(g_{k}^{h}\) is Fourier supported within the annulus \(R_{k+1}^{-1/3}\le |\xi |\le 10 R_{k}^{-1/3}\). By dyadic pigeonholing, there is some dyadic \(s\in [R_{k+1}^{-1/3},R_{k}^{-1/3}]\) for which
where \(\eta _{s}:\mathbb{R}^{3}\to [0,\infty )\) is a smooth function supported in the annulus \(s/4\le |\xi |\le s\) (in the case that \(s=R_{k}^{-1/3}\), let \(\eta _{s}\) be supported on \(s\le |\xi |\le 20R_{k}^{-1/3}\)). In the proof of Lemma 2.4, we showed the pointwise equality
where \(\tau _{s}\in{\mathbf{{S}}}(s)\) and \(\tau _{s}'\sim \tau _{s}\) means that \(\tau _{s}'\in{\mathbf{{S}}}(s)\) and \(\text{dist}(2\tau _{s},2\tau _{s}')\le 2s\). For each \(\tau _{s}\), the sub-sum on the right hand side has Fourier transform supported in \(10(\tau _{2s}-\tau _{2s})\setminus B_{s}(0)\) where \(\tau _{2s}\in{\mathbf{{S}}}(2s)\) contains \(\tau _{s}\). Now write
Perform the change of variables \(x\mapsto T^{t}x\) to get
By Proposition 3.1, we may view the sub-sums corresponding to each \(\tau _{k}\) on the right hand side of (17) as having Fourier support which is part of a tiling of the cone, after applying \(T\) and dilating by a factor of \(s^{-1}\). Therefore, we may apply the wave envelope estimate Theorem 3.3, dilated by a factor of \(s^{-1}\), to obtain
where \(\tau _{2s}``\subset "\tau '\) means that \((2s)^{-1}\cdot [ T(10\tau _{2s}-10\tau _{2s})\setminus B_{s}(0)] \subset \tau '\). It remains to undo the initial steps which allowed us to apply the wave envelope estimate for the cone. First multiply both sides of the above inequality by \(|\det T|^{-3}\). Then do the change of variables \(x\mapsto (T^{-1})^{t}x\) to obtain
where by Proposition 3.2, we identify \(\tau \in{\mathbf{{S}}}(\sigma ^{-1}s)\) with \(\tau '\in{\mathbf{{S}}}_{\sigma ^{-1} s}\) via \(s^{-1}T[(10\tau -10\tau )\setminus B_{\sigma ^{-1}s/4}(0)]\sim \tau '\) and identify \(s^{-1} T^{t}U\) with a \(V\|V_{\tau ,s^{-3}}\). Next, by Cauchy-Schwartz, since the number of \(\tau _{s}\subset \tau _{2s}\) and the number of \(\tau _{s}'\) satisfying \(\tau _{s}'\sim \tau _{s}\) is \(O(1)\), it suffices to replace the above integrals by
where . Note that \(\|\rho \|_{1}\sim 1\). Again, by Cauchy-Schwarz, the above integral is bounded by
Write \(\chi _{V_{0}}\) for the characteristic function of \(2V_{\tau ,s^{-3}}\). After summing the above integral over \(V\|V_{\tau ,s^{-3}}\), we have the bound
By Cauchy-Schwarz and Young’s convolution inequality, the right hand side is bounded by
□
4 Key iterations that unwind the pruning process
4.1 An \(L^{7/2}\) square function estimate for the parabola
Let \(\mathbb{P}^{1}=\{(t,t^{2}):0\le t\le 1\}\) and for \(r\ge 1\), let \(\mathcal {N}_{r^{-1}}(\mathbb{P}^{1})\) denote the \(r^{-1}\)-neighborhood of \(\mathbb{P}^{1}\) in \(\mathbb{R}^{2}\). Define the collection of canonical \(\sim r^{-1/2}\times r^{-1}\) parabola blocks as follows. Let \(s\in 2^{\mathbb{Z}}\) be the smallest number satisfying \(r^{-1}\le s^{2}\). Then write \(\mathcal {N}_{s^{2}}(\mathbb{P}^{1})\) as
and the two end pieces
We use the notation \(\ell (\tau )=r^{-1/2}\) in two ways: (1) to describe \(\tau \) as one of the blocks from the above partition and (2) to index the set of \(\tau \) from the above partition.
Theorem 4.1
Cylindrical \(L^{7/2}\) square function estimate over \(\mathbb{P}^{1}\)
Let \(\mathbb{P}^{1}=\{(t,t^{2}):0\le t\le 1\}\) and for \(r\ge 1\), let \(\mathcal {N}_{r^{-1}}(\mathbb{P}^{1})\) denote the \(r^{-1}\)-neighborhood of \(\mathbb{P}^{1}\) in \(\mathbb{R}^{2}\). If \(h:\mathbb{R}^{3}\to \mathbb{C}\) is a Schwartz function with Fourier transform supported in \(\mathcal {N}_{r^{-1}}(\mathbb{P}^{1})\times \mathbb{R}\), then
where the \(\zeta \) are products of approximate rectangles \(\theta \), \(\ell (\theta )={r^{-1/2}}\), with ℝ.
The local version of Theorem 4.1 is
Corollary 4.2
Let \(B_{r}\) be an \(r\)-ball in \(\mathbb{R}^{3}\). If \(h:\mathbb{R}^{3}\to \mathbb{C}\) is a Schwartz function with Fourier transform supported in \(\mathcal {N}_{r^{-1}}(\mathbb{P}^{1})\times \mathbb{R}\), then
where the \(\zeta \) are products of approximate rectangles \(\theta \), \(\ell (\theta )={r^{-1/2}}\), with ℝ.
We delay the proofs of Theorem 4.1 and Corollary 4.2 to §A.1.1 in Appendix A.
Lemma 4.3
Let \(R_{k-1}\le r\le R_{k}\). For each \(r^{-\frac{1}{3}}\le \sigma \le 1\), \(\tau \in{\mathbf{{S}}}({\sigma ^{-1}r^{-\frac{1}{3}}})\), and \(V\|V_{\tau ,r}\), we have
where \(m\ge k\) satisfies \(R_{m}^{-\frac{1}{3}}\le \sigma ^{\frac{1}{2}}r^{-\frac{1}{3}}\le R_{m-1}^{- \frac{1}{3}}\).
The weight function \(W_{V}\) is defined by \(w(T^{-1}x)\), where \(T\) is an affine transformation mapping the unit cube to \(V\) and \(w(\cdot )\) is the function from Definition 5.
Proof of Lemma 4.3
This would be a straightforward consequence of Corollary 4.2 after a moment curve rescaling, except for the fact that the pruning process alters the Fourier support of \(f\). Let \(s=\min (r^{-\frac{1}{3}},R_{m-1}^{-\frac{1}{3}})\). First we will show that
for \(R_{m}^{-\frac{1}{3}}\le \sigma ^{\frac{1}{2}}r^{-\frac{1}{3}}\le R_{m-1}^{- \frac{1}{3}}\). If \(r^{-\frac{1}{3}}\le R_{m-1}^{-\frac{1}{3}}\), then \(|f_{\tau '}^{k}|\le |f_{\tau '}^{m}|\) and (19) is trivially true, so assume that \(R_{m-1}^{-\frac{1}{3}}< r^{-\frac{1}{3}}\). This assumption also implies that \(R_{m-1}^{-\frac{1}{3}}\le R_{k}^{-\frac{1}{3}}\), so \(k< m\). We will perform an “unwinding the pruning” process using successive applications of Corollary 4.2.
Begin by performing a moment curve rescaling. Suppose that \(\tau \in{\mathbf{{S}}}(\sigma ^{-1}r^{-\frac{1}{3}})\) is the \(l\)th piece, meaning
where \(0\le l\le \sigma r^{\frac{1}{3}}-1\). Define the affine transformation \(T:\mathbb{R}^{3}\to \mathbb{R}^{3}\) by \(T(\xi _{1},\xi _{2}, \xi _{3})=(\xi _{1}',\xi _{2}',\xi _{3}')\) where
It is not difficult to verify that for each \(k\le l\le m-1\) and \(\tau _{l}\in{\mathbf{{S}}}(R_{l}^{-\frac{1}{3}})\), \(T(\tau _{l})\) is a canonical moment curve block in \({\mathbf{{S}}}(\sigma r^{\frac{1}{3}}R_{l}^{-\frac{1}{3}})\). For each \(\tau ''\in{\mathbf{{S}}}(\sigma ^{\frac{1}{2}}r^{-\frac{1}{3}})\), \(T(\tau '')\) is a canonical moment curve block in \({\mathbf{{S}}}(\sigma ^{\frac{3}{2}})\).
Let \(T(\xi )=A\xi +b\) where \(A:\mathbb{R}^{3}\to \mathbb{R}^{3}\) is a linear transformation and \(\xi ,b\in \mathbb{R}^{3}\). Perform the change of variables \(x\mapsto A^{T}x\), obtaining
Write \(f_{\tau '}^{k}\circ A^{T}=g_{T(\tau ')}^{k}\) where \(g_{T(\tau ')}^{k}\) is the Fourier projection of a Schwartz function onto \(2T(\tau ')\) (the dilation by 2 reflects the fact that \(f_{\tau '}^{k}\) is supported in \(2\tau '\)). In fact, since \(f_{\tau '}^{k}\) is Fourier supported in \(\cup _{\tau _{k}\subset \tau '}2\tau _{k}\), \(g_{T(\tau ')}^{k}\) is Fourier supported in \(\cup _{\tau _{k}\subset \tau '}2T(\tau _{k})\).
Next, consider what the set \((A^{T})^{-1}(V)\) is. The matrix representations of \(A\) and \((A^{T})^{-1}\) are
The set \(V\) is a translation of \(V_{\tau ,r}\) which is comparable to the set
where the vectors \({\mathbf{{T}}},{\mathbf{{N}}},{\mathbf{{B}}}\) are defined in (10). Using these explicit expressions, we see that \((A^{T})^{-1}(V)\) is comparable to a \(\sigma ^{-3}\)-ball in \(\mathbb{R}^{3}\).
For our first step in showing (19), we would like to apply Corollary 4.2 to estimate \(g_{T(\tau ')}^{k}\) by a square function in \(T(\tau _{k})\subset T(\tau ')\). Since \(T(\tau _{k})\) are moment curve blocks in \({\mathbf{{S}}}(\sigma r^{\frac{1}{3}}R_{k}^{-\frac{1}{3}})\), Corollary 4.2 may be employed on balls of radius \(\sigma ^{-2}r^{-\frac{2}{3}}R_{k}^{\frac{2}{3}}\). The assumptions that \(\sigma ^{\frac{1}{2}}r^{-\frac{1}{3}}\le R_{m-1}^{-\frac{1}{3}}\le R_{k}^{- \frac{1}{3}}\) mean that \(r^{-\frac{2}{3}}R_{k}^{\frac{2}{3}}\le \sigma ^{-1}\). Since \((A^{T})^{-1}(V)\) is comparable to a \(\sigma ^{-3}\)-ball which contains \(\sigma ^{-2}r^{-\frac{2}{3}}R_{k}^{\frac{2}{3}}\)-balls, Corollary 4.2 applies, yielding
Then by (1) of Lemma 2.1, \(|f_{\tau _{k}}^{k}|\le |f_{\tau _{k}}^{k+1}|\), so
If \(k+1=m\), then we are done showing (19). If \(k+1< m\), then by Khintchine’s inequality, we may select signs \(c_{\tau _{k}}\in \{\pm 1\}\) so that
The function \(\sum _{\tau _{k}\subset \tau '}c_{\tau _{k}}f_{\tau _{k}}^{k+1} \circ A^{T}=g_{T(\tau ')}^{k+1}\) where \(g_{T(\tau ')}^{k+1}\) has Fourier support in \(\cup _{\tau _{k+1}\subset \tau '}2T(\tau _{k+1})\). Then we may apply Corollary 4.2 again to obtain
Again, use \(|f_{\tau _{k+1}}^{k+1}|\le |f_{\tau _{k+2}}^{k+2}|\) and halt if \(m=k+2\) or find signs \(c_{\tau _{k+1}}\in \{\pm 1\}\) for which
Iterating this process and undoing the change of variables results in (19). Note that since \(m-k\le \varepsilon ^{-1}\), the accumulated constant satisfies \((C_{\varepsilon }R^{\varepsilon ^{9}})^{\varepsilon ^{-1}}\le C_{\varepsilon }^{\varepsilon ^{-1}}R^{\varepsilon ^{8}}\). For the final step, we perform the same argument as above, using a change of variables and Khintchine’s inequality to write
Since for \(\tau ''\in{\mathbf{{S}}}(\sigma ^{\frac{1}{2}}r^{-\frac{1}{3}})\) with \(\tau ''\subset \tau \) we have \(T(\tau '')\in{\mathbf{{S}}}(\sigma ^{\frac{3}{2}})\), we may apply Corollary 4.2 one last time to get
Finally, undo the change of variables to get
□
4.2 An \(\ell ^{7/4}\)-estimate for the cone
Let \(\Gamma =\{(\xi _{1},\xi _{2},\xi _{3})\in \mathbb{R}^{3}:\xi _{1}^{2}+\xi _{2}^{2}= \xi _{3}^{2},\quad \frac{1}{2}\le \xi _{3}\le 1\}\) be the truncated cone. In this section, let \({\mathbf{{S}}}_{r^{-1/2}}\) denote the collection of \(1\times r^{-1/2}\times r^{-1}\) blocks which tile \(\mathcal {N}_{r^{-1}}(\Gamma )\), as defined in §5 of [GM22a].
Proposition 4.4
For any Schwartz function \(h:\mathbb{R}^{3}\to \mathbb{C}\) with \(\widehat{h}\) supported in \(\mathcal {N}_{r^{-1}}(\Gamma )\), we have
We delay the proof of Proposition 4.4 to §A.2.
Lemma 4.5
For \(10\le r_{1}\le r_{2}\) and \(R_{k-1}\le r_{2}\le R_{k}\), there exists some dyadic \(s\), \(R^{-\frac{1}{3}}\le s\le r_{2}^{-\frac{1}{3}}\) such that
where \(k_{m}\ge k\) satisfies \(R_{k_{m}}^{-\frac{1}{3}}\le s\le R_{k_{m}-1}^{-\frac{1}{3}}\).
Proof of Lemma 4.5
Fix a \(\tau _{0}\) and analyze each integral on the left hand side of (20). Suppose that there is some dyadic value \(s\) in the range \(R_{k}^{-1/3}\le s\le r_{2}^{-1/3}\) which satisfies
The next step repeats the argument from Lemma 3.4, which we provide a sketch for now. By the proof of Lemma 3.2, the integral on the right hand side above is equivalent to
where \(\tau _{s}'\sim \tau _{s}\) means that \(\text{dist}(\tau _{s}',\tau _{s})\lesssim s\). By Propositions 3.1 and 3.2, the Fourier support of the integrand may now be viewed as a canonical tiling of (an \(s\)-dilation of) the cone. Therefore, we may apply Proposition 4.4 to bound the previous displayed integral by
where we are free to choose \(\delta >0\). Here, the iteration ends since we have proven the lemma.
In the case that (21) does not hold, we may assume that
Applying the argument from Lemma 2.4 to the integrand, we have
Since is \(L^{1}\)-normalized, we may ignore the by Young’s convolution inequality. Then by Lemma 2.1, we have the pointwise inequality \(|f_{\tau _{k}}^{k}|\le |f_{\tau _{k}}^{k+1}|\). The conclusion in this case is that
Next, we iterate this procedure, considering the two cases (21) and (22) applied to the integral on the right hand side above. The number of steps in the iteration is the same as the number of times (the appropriate version of) (22) holds. Each time (22) holds, we refine the scale of our square function by a factor of \(R^{\varepsilon /3}\) (moving from \(\tau _{k}\) to \(\tau _{k+1}\), say). Therefore, the total number of steps is bounded by \(\varepsilon ^{-1}\). In the case that (21) holds at one step, the iteration terminates with an accumulated constant of at most \((\log R)^{\varepsilon ^{-1}}B_{\delta }R^{\delta \varepsilon ^{-1}}\). Since we are free to choose \(\delta \), this proves the proposition. The final case is that (22) holds at all steps in the iteration. This leads to the first term from the upper bound in (20). □
4.3 Algorithm to fully unwind the pruning process
Recall some notation which was defined in §3.
-
(1)
For each dyadic \(\sigma \), \(R_{k}^{-\frac{1}{3}}\sigma \le 1\) and each \(\tau \in{\mathbf{{S}}}(\sigma ^{-1}R_{k}^{-\frac{1}{3}})\), the dual set \(\tau ^{*}\) is a \(\sigma R_{k}^{\frac{1}{3}}\times \sigma ^{2}R_{k}^{\frac{2}{3}} \times \sigma ^{3}R_{k}\) plank centered at the origin and comparable to \(\{x\in \mathbb{R}^{3}:|x\cdot \xi |\le 1\qquad \forall \xi \in \tau -\tau \}\). The wave envelope \(V_{\tau ,R_{k}}\) is an anisotropically dilated version of \(\tau ^{*}\) with dimensions \(\sigma ^{-2}R_{k}^{-\frac{1}{3}}\times \sigma ^{-1}R_{k}^{- \frac{2}{3}}\times R_{k}^{-1}\).
-
(2)
Let \(V\|V_{\tau ,R_{k}}\) denote an indexing set for \(V\) which are translates of \(V_{\tau ,R_{k}}\) and which tile \(\mathbb{R}^{3}\).
Proposition 4.6
For each \(k\), we have
Propositon 4.6 will follow from an algorithm which uses the Lemmas 4.3 and 4.5 as building blocks.
Proof of Proposition 4.6
Let \(C>0\) be an absolute constant that we specify later in the proof. We will define an algorithm which at intermediate step \(m\), produces an inequality
in which \(a+b=m\) and \(R^{-\frac{1}{3}}\le s_{m}\le R_{k}^{-\frac{1}{3}}R^{- \frac{\varepsilon ^{3}}{2}a}R^{-\frac{\varepsilon }{3}b}\) and \(k_{m}\ge k+1\) satisfies \(R_{k_{m}}^{-\frac{1}{3}}\le s_{m}\le R_{k_{m}-1}^{-\frac{1}{3}}\). Notice that (24) clearly holds with \(m=0\), taking \(k_{m}=k+1\) and \(s_{m}=R_{k}^{-\frac{1}{3}}\). Assuming (24) holds for \(m-1\), we will show that either the algorithm terminates and the proposition is proved or (24) holds for \(m\ge 1\). We further suppose that \(R^{-\frac{1}{3}}R^{\frac{\varepsilon }{3}}\le s_{m-1}\), otherwise proceed to the final case in which the algorithm terminates below.
Step m: Let \(\sigma \in [s_{m-1},1]\) be a dyadic value satisfying
The analysis splits into two cases depending on whether \(\sigma \ge R^{-\varepsilon ^{3}}\) or \(\sigma < R^{-\varepsilon ^{3}}\).
Step m: \(\sigma \ge R^{-\varepsilon ^{3}}\). Using Cauchy-Schwarz and then Hölder’s inequality, for each \(\tau \in{\mathbf{{S}}}(\sigma ^{-1}s_{m-1})\),
Define \(k_{m-1}^{*}\) to be \(k_{m-1}^{*}=k_{m-1}+1\) if \(s_{m-1}=R_{k_{m-1}}^{-\frac{1}{3}}\) and \(k_{m-1}^{*}=k_{m-1}\) if \(R_{k_{m-1}}^{-\frac{1}{3}}< s_{m-1}\). Note that by (1) of Lemma 2.1, for each \(\tau '\in{\mathbf{{S}}}(s_{m-1})\), \(|f_{\tau '}^{k_{m-1}}|\le |f_{\tau '}^{k_{m-1}^{*}}|\). By rescaling for the moment curve, for each \(\tau '\in{\mathbf{{S}}}(s_{m-1})\),
where we used the definitions of \(\text{S}_{1}(\cdot )\) and \(\text{S}_{2}(\cdot )\) and the relationship \(\text{S}_{2}(\cdot )\lesssim \text{S}_{1}(\cdot )\), which follows from Lemma 2.2. If \(k_{m-1}^{*}=N\), then the algorithm terminates with the inequality
in which \(a+b=m-1\) and \(R^{-\frac{1}{3}}\le R_{k}^{-\frac{1}{3}}R^{-\frac{\varepsilon ^{3}}{2}a}R^{- \frac{\varepsilon }{3}b}\). If \(k_{m-1}^{*}< N\), by Lemma 4.5, there are two further cases. One case is that
and the algorithm terminates with the inequality
in which \(a+b=m-1\) and \(R^{-\frac{1}{3}}\le R_{k}^{-\frac{1}{3}}R^{-\frac{\varepsilon ^{3}}{2}a}R^{- \frac{\varepsilon }{3}b}\). We will verify further below that these termination conditions prove the proposition.
The other case from Lemma 4.5 is that there is some dyadic value \(s_{m}\), \(R^{-\frac{1}{3}}\le s_{m}\le R_{k_{m-1}^{*}}^{-\frac{1}{3}}\), which satisfies
where \(k_{m}\ge k_{m-1}^{*}\) satisfies \(R_{k_{m}}^{-\frac{1}{3}}\le s_{m}\le R_{k_{m}-1}^{-\frac{1}{3}}\). By definition of \(k_{m-1}^{*}\), \(R_{k_{m-1}^{*}}^{-\frac{1}{3}}< s_{m-1}\). Then since \(s_{m}\le R_{k_{m-1}^{*}}^{-\frac{1}{3}}< s_{m-1}\le R_{k}^{- \frac{1}{3}}R^{-\frac{\varepsilon }{3}b}\), \(R_{k_{m-1}}=R^{k_{m-1}\varepsilon }\), and \(R_{k}R^{\varepsilon b}=R^{(k+b)\varepsilon }\), it follows that \(s_{m}\le R_{k}^{-\frac{1}{3}}R^{-\frac{\varepsilon }{3}(b+1)}\). We have shown in this case that
in which \(a+(b+1)=m+1\) and \(R^{-\frac{1}{3}}\le s_{m}\le R_{k}^{-\frac{1}{3}}R^{- \frac{\varepsilon ^{3}}{2}a}R^{-\frac{\varepsilon }{3}(b+1)}\) and \(k_{m}\ge k+1\) satisfies \(R_{k_{m}}^{-\frac{1}{3}}\le s_{m}\le R_{k_{m}-1}^{-\frac{1}{3}}\), which verifies (24).
Step m: \(s_{m-1}\le \sigma \le R^{-\varepsilon ^{3}}\). Let \(\tilde{s}_{m-1}=\max (R^{-\frac{1}{3}},\sigma ^{\frac{1}{2}}s_{m-1})\). By Lemma 4.3, for each \(\tau \in{\mathbf{{S}}}(\sigma ^{-1}s_{m-1})\) and \(V\|V_{\tau ,s_{m-1}^{-3}}\),
where \(k_{m}'\ge k+1\) satisfies \(R_{k_{m}'}^{-\frac{1}{3}}\le \tilde{s}_{m-1}\le R_{k_{m}'-1}^{- \frac{1}{3}}\). Then using \(\|\cdot \|_{\ell ^{7/4}}\le \|\cdot \|_{\ell ^{1}}\) and Cauchy-Schwarz, we have
If \(\tilde{s}_{m-1}=R^{-\frac{1}{3}}\), then the algorithm terminates with the inequality
in which \(a+b=m-1\) and \(R^{-\frac{1}{3}} \le R_{k}^{-\frac{1}{3}}R^{-\frac{\varepsilon ^{3}}{2}a}R^{- \frac{\varepsilon }{3}b}\). Otherwise, suppose that \(\tilde{s}_{m-1}>R^{-\frac{1}{3}}\) and apply Lemma 4.5, again leading to two cases. In the case that
then the algorithm terminates with the same inequality as is recorded in (28).
The other case from Lemma 4.5 is that there is some dyadic value \(s_{m}\), \(R^{-\frac{1}{3}}\le s_{m}\le \sigma ^{\frac{1}{2}}s_{m-1}\), which satisfies
where \(k_{m}\ge k_{m-1}^{*}\) satisfies \(R_{k_{m}}^{-\frac{1}{3}}\le s_{m}\le R_{k_{m}-1}^{-\frac{1}{3}}\). Since \(s_{m-1}\le R_{k}^{-\frac{1}{3}}R^{-\frac{\varepsilon ^{3}}{2}a}R^{- \frac{\varepsilon }{3}b}\) and \(s_{m}\le \sigma ^{\frac{1}{2}}s_{m-1}\), we have \(s_{m}\le R_{k}^{-\frac{1}{3}}R^{-\frac{\varepsilon ^{3}}{2}(a+1)}R^{- \frac{\varepsilon }{3}b}\). We have shown in this case that
in which \((a+1)+b=m+1\) and \(R^{-\frac{1}{3}}\le s_{m}\le R_{k}^{-\frac{1}{3}}R^{- \frac{\varepsilon ^{3}}{2}(a+1)}R^{-\frac{\varepsilon }{3}b}\) and \(k_{m}\ge k+1\) satisfies \(R_{k_{m}}^{-\frac{1}{3}}\le s_{m}\le R_{k_{m}-1}^{-\frac{1}{3}}\), which verifies (24).
Termination criteria. It remains to check that the criteria for termination from both of the above cases implies Proposition 4.6. The first case in which the algorithm terminates is (27). Then \(R^{-\frac{1}{3}}\le R_{k}^{-\frac{1}{3}}R^{-\frac{\varepsilon ^{3}}{2}a}R^{- \frac{\varepsilon }{3}b})\) implies that \(a\le \frac{2}{3}\varepsilon ^{-3}(N-k)\) and \(b\le N-k\), which implies that \(m-1=a+b\le \varepsilon ^{-3}(N-k)\). Then the constants in the upper bound from (27) are bounded by
The second case in which the algorithm terminates with (28) proves the proposition by an analogous argument. □
5 Bounding the broad part of \(U_{\alpha ,\beta }\)
For three canonical blocks \(\tau ^{1},\tau ^{2},\tau ^{3}\) (with dimensions \(\sim R^{-\varepsilon /3}\times R^{-2\varepsilon /3}\times R^{-\varepsilon }\)) which are pairwise \(\ge R^{-\varepsilon /3}\)-separated, define the broad part of \(U_{\alpha ,\beta }\) to be
We bound the broad part of \(U_{\alpha ,\beta }\) in the following proposition. Recall that the parameter \(N_{0}\) was used in the definition of the sets \(\Omega _{k}\) and \(L\).
Proposition 5.1
Let \(R,K\ge 1\). Suppose that \(\|f_{\theta}\|_{L^{\infty}(\mathbb{R}^{3})}\le 2\) for all \(\theta \in{\mathbf{{S}}}(R^{-\frac{1}{3}})\). Then
We will use the following version of a local trilinear restriction inequality for the moment curve, which was proved in Proposition 6 of [GM22b]. The weight function \(W_{B_{r}}\) in the following theorem decays by a factor of 10 off of the ball \(B_{r}\). It is defined right after Definition 5.
Theorem 5.2
Let \(s\ge 10r\ge 10\). Suppose that \(\tau ^{1},\tau ^{2},\tau ^{3}\in{\mathbf{{S}}}(R^{-\varepsilon /3})\) satisfy \(\textit{dist}(\tau ^{i},\tau ^{j})\ge s^{-1}\) for \(i\neq j\). Then
for any Schwartz function \(f:\mathbb{R}^{3}\to \mathbb{C}\) with Fourier transform supported in \(\mathcal {M}(r^{3})\).
Proof of Proposition 5.1
Note that
We bound each of the sets \(\text{Br}_{\alpha ,\beta }^{K}\cap \Omega _{k}\) and \(\text{Br}_{\alpha ,\beta }^{K}\cap L\) in separate cases. It suffices to consider the case that \(R\) is at least some constant depending on \(\varepsilon \) since if \(R\le C_{\varepsilon }\), we may prove the proposition using trivial inequalities.
Case 1: bounding \(| \text{Br}_{\alpha ,\beta }^{K}\cap \Omega _{k}|\). By Lemma 2.6,
By Lemma 2.1, the Fourier supports of \(f_{\tau ^{1}}^{k+1},f_{\tau ^{2}}^{k+1},f_{\tau ^{3}}^{k+1}\) are contained in \(2\tau ^{1},2 \tau ^{2}, 2\tau ^{3}\) respectively, which are \(\ge 5 R^{-\frac{\varepsilon }{3}}\)-separated blocks of the moment curve. Let \(\{B_{R_{k}^{\frac{1}{3}}}\}\) be a finitely overlapping cover of \(\text{Br}_{\alpha ,\beta }^{K}\cap \Omega _{k}\) by \(R_{k}^{\frac{1}{3}}\)-balls. For \(R\) large enough depending on \(\varepsilon \), apply Theorem 5.2 to get
Using local \(L^{2}\)-orthogonality (Lemma 2.3), each integral on the right hand side above is bounded by
If \(x\in \text{Br}_{\alpha ,\beta }^{K}\cap \Omega _{k}\cap B_{R_{k}^{\frac{1}{3}}}\), then the above integral is bounded by
by the locally constant property (Lemma 2.2) and properties of the weight functions. The summary of the inequalities so far is that
where \(x\in \text{Br}_{\alpha ,\beta }^{K}\cap \Omega _{k}\cap B_{R_{k}^{\frac{1}{3}}}\).
Recall that since \(x\in \Omega _{k}\), we have the lower bound \(A^{M-k}\beta \le g_{k}(x)\) (where \(A\) is from Definition 8), which leads to the inequality
By Corollary 2.5, we also have the upper bound \(|g_{k}(x)|\le 2|g_{k}^{h}(x)|\), so that
By the locally constant property applied to \(g_{k}^{h}\), \(|g_{k}^{h}|^{4}\lesssim _{\varepsilon }|g_{k}^{h}*w_{ B_{R_{k}^{\frac{1}{3}}}}|^{4}\) and by Cauchy-Schwarz, \(|g_{k}^{h}*w_{ B_{R_{k}^{\frac{1}{3}}}}|^{4}\lesssim |g_{k}^{h}|^{4}*w_{B_{R_{k}^{ \frac{1}{3}}}}\). Combine this with the previous displayed inequality to get
Summing over the balls \(B_{R_{k}^{\frac{1}{3}}}\) in our finitely-overlapping cover of \(\text{Br}_{\alpha ,\beta }^{K}\cap \Omega _{k}\), we conclude that
We are done using the properties of the set \(\text{Br}_{\alpha ,\beta }^{K}\cap \Omega _{k}\), which is why we now integrate over all of \(\mathbb{R}^{3}\) on the right hand side. We will now use Lemma 3.4 to analyze the high part \(g_{k}^{h}\). In particular, Lemma 3.4 gives
Next use (2) from Lemma 2.1 to note that \(\|f_{\tau _{k}}^{k+1}\|_{\infty}\le \sum _{\tau _{k+1}\subset \tau _{k}} \|f_{\tau _{k+1}}^{k+1}\|_{\infty}\lesssim R^{\varepsilon }A^{\varepsilon ^{-1}}K^{3} \frac{\beta }{\alpha }\): for each \(R_{k}^{-1/3}\le \sigma \le 1\), \(\tau \in{\mathbf{{S}}}(\sigma ^{-1}R_{k}^{-\frac{1}{3}})\) and \(V\|V_{\tau ,R_{k}}\),
Using this and applying Proposition 4.6 gives the upper bound
Combining this with (29) and (30), the summary of the argument from this case is
Since \(k>N_{0}\), this upper bound has the desired form.
Case 2: bounding \(|U_{\alpha ,\beta }\cap L|\). Begin by using Lemma 2.6 to bound
Then use Cauchy-Schwarz and the locally constant property for \(g_{N_{0}}\):
Using the definition the definition of \(L\), we bound the factors of \(g_{N_{0}}\) by
Finally, by the definition of \(U_{\alpha ,\beta }\), conclude that
□
6 Proof of Theorem 1 from Proposition 5.1
First, we prove Proposition 6.1 below, which is that \(\text{S}_{1}(R)\lesssim _{\varepsilon }R^{\varepsilon }\). This follows using various reductions from pigeonholing, a broad-narrow argument, and the broad estimate Proposition 5.1. Then, in §6.3, we use induction to show that Proposition (6.1) implies that \(\text{S}_{2}(R)\lesssim _{\varepsilon }R^{\varepsilon }\), which is equivalent to Theorem 1.
Proposition 6.1
For any \(\varepsilon >0\) and \(R\ge 1\),
In order to make use of Proposition 5.1, we need to reduce to the case that our function \(f\) is localized to a ball, its wave packets have been pigeonholed so that \(\|f_{\theta}\|_{\infty}\lesssim 1\) for all \(\theta \in{\mathbf{{S}}}(R^{-1/3})\), and we have approximated \(\|f\|_{7}\) by an expression involving a superlevel set. This is the content of the following subsection.
6.1 Wave packet decomposition and pigeonholing
Begin with the spatial localization.
Lemma 6.2
For any \(R\)-ball \(B_{R}\subset \mathbb{R}^{3}\), suppose that
for any Schwartz function \(f:\mathbb{R}^{3}\to \mathbb{C}\) with Fourier transform supported in \(\mathcal {M}^{3}(R)\). Then Proposition 6.1is true.
Proof
If \(\phi _{B_{R}}\) is a Schwartz function that rapidly decays away from \(B_{R}\), has Fourier transform supported in \(B_{R^{-1}}(0)\), and satisfies \(\phi _{B_{R}}\gtrsim 1\) on \(B_{R}\), then we may apply the hypothesis to the function \(\phi _{B_{R}}f\) to obtain
where the sum is over a finitely overlapping cover of \(\mathbb{R}^{3}\) by \(R\)-balls. Then, since \(\|\cdot \|_{\ell ^{7/2}}\le \|\cdot \|_{\ell ^{1}}\),
It remains to note that \(\sum _{B_{r}}|\phi _{B_{r}}|^{2}\lesssim 1\). □
It further suffices to prove a weak, level-set version of Proposition 6.1.
Lemma 6.3
For each \(B_{R}\) and Schwartz function \(f:\mathbb{R}^{3}\to \mathbb{C}\) with Fourier transform supported in \(\mathcal {M}^{3}(R)\), there exists \(\alpha >0\) such that
Proof
Split the integral as follows:
in which \(\lambda \) varies over dyadic values in the range \([R^{-1000},1]\). If one of the \(\lesssim \log R\) many terms in the first sum dominates, then we are done. Suppose instead that the second expression dominates:
We have
□
Continue to use the notation
We will show that to estimate the size of \(U_{\alpha }\), it suffices to replace \(f\) with a version whose wave packets at scale \(\theta \) have been pigeonholed. Write
where for each \(\theta \in{\mathbf{{S}}}(R^{-1/3})\), \(\{\psi _{T}\}_{T\in \mathbb{T}_{\theta}}\) is the partition of unity from §2.1. If \(\alpha \le C_{\varepsilon }R^{-100}\max _{\theta}\|f_{\theta}\|_{\infty}\), then using a similar argument that bounds the second expression in the proof of Lemma 6.3, the inequality
is trivial.
Proposition 6.4
Wave packet decomposition
Let \({\alpha }>C_{\varepsilon }R^{-100}\max _{\theta}\|f_{\theta}\|_{L^{\infty}(\mathbb{R}^{3})}\). There exist subsets \(\tilde{\mathbb{T}}_{\theta}\subset \mathbb{T}_{\theta}\), as well as a constant \(A>0\) with the following properties:
Proof
Split the sum (31) into
where the close set is
and the far set is
Using the rapid decay of the partition of unity, for each \(x\in U_{ {\alpha }}\),
Therefore, using the assumption that \({{\alpha }}\) is at least \(C_{\varepsilon }R^{-100}\max _{\theta}\|f_{\theta}\|_{L^{\infty}(\mathbb{R}^{3})}\),
Now we sort the close wave packets according to amplitude. Let
Split the remaining wave packets into
where \(\lambda \) is a dyadic number in the range \([R^{-10^{3}},1]\),
and
Again using the lower bound for \({\alpha }\) (and the fact that the number of \(T\in \mathbb{T}_{\theta}^{c}\) is bounded by \(R^{4}\)), the small wave packets cannot dominate and we have
By dyadic pigeonholing, for some \(\lambda \in [R^{-1000},1]\),
Note that we have the pointwise inequality
We know that \(\lambda M\ge C_{\varepsilon }R^{-1000}\max _{\theta}\|f_{\theta}\|_{L^{\infty}( \mathbb{R}^{3})}\) since if this did not hold, we would violate the lower bound for \(\alpha \). It follows that
The statement of the lemma is now satisfied with \(A=\lambda M\) and \(\tilde{\mathbb{T}}_{\theta}=\mathbb{T}_{\theta ,\lambda}^{c}\). □
Corollary 6.5
Let \(f\), \(\alpha \), \(\tilde{\mathbb{T}}_{\theta}\) and \(A>0\) be as in Proposition 6.4. Then for each \(x\in U_{\alpha }\),
Proof
Let \(x\in U_{\alpha }\). Then using the rapid decay of \(\psi _{T}\) off of \(T\),
Then the lower bound for \(\alpha \) and (35) imply that
By the locally constant property, if \(\eta _{\theta}\) is a standard bump function equal to 1 on \(\theta \), then
for some \(z_{\theta}\in \mathbb{R}^{3}\). Note that if either \(y\notin \frac{1}{2}R^{\varepsilon }T\) or \(z_{\theta}-y\notin \frac{1}{2}R^{\varepsilon }\theta ^{*}\), then . It follows from the lower bound on \(\alpha \) that
It remains to note that for each \(\theta \) counted on the right hand side above, and for each \(y\in R^{\varepsilon }T\), . □
Lemma 6.6
For each \(\alpha >0\), \(B_{R}\), and Schwartz function \(f:\mathbb{R}^{3}\to \mathbb{C}\) with Fourier transform supported in \(\mathcal {M}^{3}(R)\), there exists \(\beta >0\) such that \(\alpha ^{7}|\{x\in B_{R}:\alpha \le |f(x)|\}|\) is bounded by
Proof
First fix the notation
and \(g=\sum _{\theta \in{\mathbf{{S}}}(R^{-1/3})}|f_{\theta}|^{2}*\omega _{\theta}\). Then write
where \(\lambda \) takes dyadic values and \(g(x)\sim \lambda \|g\|_{L^{\infty}(B_{R})}\) means \(\lambda \|g\|_{L^{\infty}(B_{R})}/2\le g(x)\le \lambda \|g\|_{L^{ \infty}(B_{R})}\). If one of the first \(\le C(\log R)\) terms dominates the sum, then the lemma is proved. Suppose instead that the last term dominates, so that
Then
□
6.2 A multi-scale inequality for \(\text{S}_{1}(R)\) implying Proposition 6.1
First we use a broad/narrow analysis to prove a multi-scale inequality for \(\text{S}_{1}(R)\).
Lemma 6.7
For any \(1\le K^{3}\le R\) and \(1\le N_{0}\le \varepsilon ^{-1}\),
Proposition 5.1 implies Lemma 6.7
Let \(f:\mathbb{R}^{3}\to \mathbb{C}\) be a Schwartz function with Fourier transform supported in \(\mathcal {M}^{3}(R)\). By Lemma 6.2, it suffices to bound \(\|f\|_{L^{7}(B_{R})}^{7}\) instead of \(\|f\|_{L^{7}(\mathbb{R}^{3})}^{7}\). By Lemma 6.3, we may fix \(\alpha >0\) so that \(\|f\|_{L^{7}(B_{R})}^{7}\lesssim (\log R)^{2}\alpha ^{7}|U_{\alpha }|\). By Proposition 6.4, we may replace \(\alpha \) by \(\alpha /A\) and replace \(f\) by \(\tilde{f}=\frac{1}{A}\sum _{\theta \in{\mathbf{{S}}}(R^{-1/3})}\sum _{T \in \tilde{\mathbb{T}}_{\theta}} \psi _{T}f_{\theta}\) where \(\tilde{\mathbb{T}}_{\theta}\) satisfies the properties in that proposition. From here, we will take \(f\) to mean \(\tilde{f}\). By Lemma 6.6, we may fix \(\beta >0\) so that \(\alpha ^{7}|U_{\alpha }|\lesssim (\log R)\alpha ^{7}|U_{\alpha ,\beta }|\). Finally, by Corollary 6.5, we have \(\alpha \lesssim R^{103}\).
Write \(f=\sum _{\tau \in{\mathbf{{S}}}(K^{-1})}f_{\tau}\). The broad-narrow inequality is
Indeed, suppose that the set \(\{\tau \in{\mathbf{{S}}}(K^{-1}):|f_{\tau}(x)|\ge K^{-1}\max _{\tau '\in{ \mathbf{{S}}}(K^{-1})}|f_{\tau '}(x)|\}\) has at least 5 elements. Then we can find three \(\tau ^{1},\tau ^{2},\tau ^{3}\) which are pairwise \(\ge K^{-1}\)-separated and satisfy \(|f(x)|\le K^{3}|f_{\tau ^{1}}(x)f_{\tau ^{2}}(x)f_{\tau ^{3}}(x)|^{ \frac{1}{3}}\). If there are fewer than 5 elements, then \(|f(x)|\le 6 \max _{\tau \in{\mathbf{{S}}}(K^{-1})}|f_{\tau}(x)|\).
The broad-narrow inequality leads to two possibilities. In one case, we have
Then the summary of inequalities from this case is
By rescaling for the moment curve and the definition of \(\text{S}_{1}(\cdot )\), we may bound each integral in the final upper bound by
Noting that \(\sum _{\tau}\int _{\mathbb{R}^{3}}|\sum _{\theta \subset \tau}|f_{\theta}|^{2}* \omega _{\theta}|^{7/2}\le \int _{\mathbb{R}^{3}}|\sum _{\theta}|f_{\theta}|^{2}* \omega _{\theta}|^{7/2} \) finishes this case.
The remaining case from the broad-narrow inequality is that
We may further assume that
since otherwise, we would be in the first case (40). The size of the set above is now bounded by a sum over pairwise \(K^{-1}\)-separated 3-tuples \((\tau ^{1},\tau ^{2},\tau ^{3})\) of \(|\text{Br}_{\alpha ,\beta }^{K}|\) from §5. Using Proposition 5.1 to bound \(|\text{Br}_{\alpha ,\beta }^{K}|\), the summary of the inequalities from this case is
which finishes the proof. □
With Lemma 6.7 in hand, we may now prove Proposition 6.1.
Proof of Proposition 6.1
Let \(\eta \) be the infimum of the set
Suppose that \(\eta >0\). Let \(\varepsilon _{1}\), \(\eta >\varepsilon _{1}>0\), be a parameter we will specify later. By Lemma 6.7, we have
where we are free to choose \(\varepsilon >0\), \(1\le N_{0}\le \varepsilon ^{-1}\), and \(1\le K^{3}\le R\). Continue to bound the expression on the right hand side by
By definition of \(\eta \),
so it suffices to check that
to obtain a contradiction. From here, choose \(N_{0}=\varepsilon ^{-1/2}\) and \(K=R^{\varepsilon _{1}}\) so that it suffices to check
This is clearly true if we choose \(\varepsilon >0\) to satisfy \(\min (\eta -10\varepsilon ^{1/2},\eta -4\varepsilon ^{3/2}-10\varepsilon ^{1/2})>\eta /2\) and then choose \(\varepsilon _{1}\) to be smaller than \(\frac{1}{55}\varepsilon ^{1/2}\eta /4\). Our reasoning has shown that \(\eta -\varepsilon _{1}\in \mathcal {S}\), which is a contradiction. Conclude that \(\eta =0\), as desired. □
6.3 Proof of Theorem 1
We will show that \(\text{S}_{1}(R)\lesssim _{\varepsilon }R^{\varepsilon }\) implies \(\text{S}_{2}(R)\lesssim _{\varepsilon }R^{\varepsilon }\), which proves Theorem 1. See Definitions 1 and 2 in §1.2 for the definitions of \(\text{S}_{1}(R)\) and \(\text{S}_{2}(R)\).
The following is a multi-scale inequality relating \(\text{S}_{1}(R)\) to \(\text{S}_{2}(\cdot )\) and \(\text{S}_{1}(\cdot )\) evaluated at parameters smaller than \(R\).
Proposition 6.8
For \(R\ge 10\),
Granting this proposition, we now prove Theorem 1.
Proof of Theorem 1
Let \(\eta \) be the infimum of the set
Suppose that \(\eta >0\). Let \(\varepsilon _{1}>0\) satisfy \((1/3)\eta -\varepsilon _{1}>0\). By Proposition 6.8, we have
where \(\delta \) is any positive number in the last line. By definition of \(\eta \),
Therefore,
Choose \(\delta >0\) so that \((1/3)\eta -\varepsilon _{1}-(2/3)\delta >0\). Then choose \(\varepsilon >0\) so that \((1/3)\eta -\varepsilon _{1}-(2/3)\delta -\varepsilon >0\). Since by Proposition 6.1, we know that \(\text{S}_{1}(R)\) grows slower than any power in \(R\), conclude that
The sequence of inequalities shows that \(\eta -\varepsilon _{1}\in{ \mathcal {S}}\), which contradicts the fact that \(\eta \) is the infimum. Conclude that \(\eta =0\). □
It remains to prove Proposition 6.8, which we do presently.
Proof of Proposition 6.8
Let \(f:\mathbb{R}^{3}\to \mathbb{C}\) be a Schwartz function with Fourier transform supported in \(\mathcal {M}^{3}(R)\). Begin with the defining inequality for \(\text{S}_{1}(R^{1/3})\):
We choose the scale \(R^{1/3}\) because each \(\omega _{\tau}\) is localized to an \(R^{1/9}\times R^{2/9}\times R^{1/3}\) plank, which is contained in an \(R^{1/3}\) ball. The square function we are aiming for, \(\sum _{\theta \in{\mathbf{{S}}}(R^{-1/3})}|f_{\theta}|^{2}\), is locally constant on \(R^{1/3}\) balls, so we will be able to eliminate the weights and therefore obtain a bound for \(\text{S}_{2}(R)\). The idea for going from the right hand side of (41) to our desired right hand side is to perform an algorithm similar to Proposition 4.6. We may vastly simplify the process since here we have not performed any pruning steps which give \(k\)th versions of \(f\) with altered Fourier support.
Begin with the assumption that
Indeed, if this does not hold, then we may assume
Then we have reached our termination criterion since by local \(L^{2}\)-orthogonality, for each \(\tau \in{\mathbf{{S}}}(R^{-1/9})\),
Finally, simply note that and by Young’s convolution inequality,
From here on, assume that (42) holds.
Now we describe the simplified algorithm. Let \(\delta >0\) be a constant that we specify later in the proof. At intermediate step \(m\), we have the inequality
in which \(R^{-\frac{1}{3}}\le s_{m}\le R^{-\frac{1}{9}}R^{-\frac{\varepsilon ^{2}}{2}m}\). We begin by showing that (43) holds with \(m=1\).
Step 1: The Fourier support of is in the annulus \(\{R^{-1/3}\le |\xi |\le 2R^{-1/9}\}\). Since \(\sum _{\substack{R^{-1/3}\le s\le 3R^{-1/9}}}\eta _{s}\equiv 1\) (where \(s\) takes dyadic values) on this annulus, there is some dyadic \(s_{1}\), \(R^{-1/3}\le s_{1}\le 3R^{-1/9}\) such that
By pointwise local \(L^{2}\)-orthogonality (or the proof of Lemma 2.4),
where \(\tau '\sim \tau ''\) means \(d(\tau ',\tau '')\le 3 s_{1}\). For each \(\tau \in{\mathbf{{S}}}(R^{-1/9})\) and \(\tau '\subset \tau \), \(\tau '\in{\mathbf{{S}}}(s_{1})\), the Fourier support of
is contained in \((10\tau '-10\tau ')\setminus B_{s_{1}}\), which, after dilating by a factor of \(s_{1}^{-1}\), we may identify with a conical cap as we did in §3. Therefore, we may apply Proposition 4.4 (with space rescaled by a factor of \(s_{1}^{-1}\)) to obtain
For each \(s_{1}\le \sigma \le 1\), \(\underline {\tau}\in{\mathbf{{S}}}(\sigma ^{-1}s_{1})\), and \(V\|V_{\underline {\tau},s_{1}^{-3}}\), by Cauchy-Schwarz and Hölder’s inequality,
Note that since \(\tau '\subset \tau \), we have \(\tau ^{*}\subset 2(\tau ')^{*}\) and each \((\tau ')^{*}\subset 2V_{\tau ,s_{1}^{-3}}\). Also note that \(B_{s_{1}}(0)\subset V_{\tau ,s_{1}^{-3}}\). By properties of weight functions, it follows that
This concludes Step 1.
From here, we assume that for \(m>1\), Step \(m-1\) holds. We will show that either the algorithm terminates with the desired inequality or Step \(m\) (i.e. (43)) holds.
Step m: Let \(\sigma \in [s_{m-1},1]\) be a dyadic value satisfying
The analysis splits into two cases depending on whether \(\sigma \ge R^{-\varepsilon ^{2}}\) or \(\sigma < R^{-\varepsilon ^{2}}\).
Step m: \(\sigma \ge R^{-\varepsilon ^{2}}\). Using Cauchy-Schwarz and then Hölder’s inequality, for each \(\tau \in{\mathbf{{S}}}(\sigma ^{-1}s_{m-1})\),
By rescaling for the moment curve, for each \(\tau '\in{\mathbf{{S}}}(s_{m-1})\),
Since \(\sum _{\tau '\in{\mathbf{{S}}}(\sigma ^{-1}s_{m-1})}\int _{\mathbb{R}^{3}}(\sum _{ \theta \subset \tau '}|f_{\theta}|^{2})^{7/2}\le \int _{\mathbb{R}^{3}}( \sum _{\theta}|f_{\theta}|^{2})^{7/2}\), the algorithm terminates in this case with the inequality
Step m: \(s_{m-1}\le \sigma \le R^{-\varepsilon ^{2}}\). Let \(\tilde{s}_{m-1}=\max (R^{-\frac{1}{3}},\sigma ^{\frac{1}{2}}s_{m-1})\). By Lemma 4.3 (which applies equally well to functions which have not been pruned), for each \(\tau \in{\mathbf{{S}}}(\sigma ^{-1}s_{m-1})\) and \(V\|V_{\tau ,s_{m-1}^{-3}}\),
Then using \(\|\cdot \|_{\ell ^{7/4}}\le \|\cdot \|_{\ell ^{1}}\) and Cauchy-Schwarz, we have
If \(\tilde{s}_{m-1}=R^{-\frac{1}{3}}\), then the algorithm terminates with the inequality
Otherwise, suppose that \(\tilde{s}_{m-1}>R^{-\frac{1}{3}}\). Then the inequality so far reads
By the same reasoning as in Step 1, either we are in a termination case analogous to when (42) does not hold, or there is some \(s_{m}\le \sigma ^{\frac{1}{2}}s_{m-1}\) for which
By the hypothesis that \(s_{m-1}\le R^{-\frac{1}{9}}R^{\frac{-\varepsilon ^{2}}{2}(m-1)}\) and \(\sigma \le R^{-\varepsilon ^{2}}\), we have \(s_{m}\le R^{-\frac{1}{9}}R^{\frac{-\varepsilon ^{2}}{2}m}\). This completes the justification of Step \(m\).
Termination criteria. It remains to summarize the termination criteria. In each of the termination scenarios, if \(\text{S}_{2}(\cdot )\) appears, then it is multiplied by one factor of \(R^{\varepsilon ^{2}}\) and is evaluated at some parameter \(\lambda \) between 1 and \(R^{2/3}\). Finally, consider the accumulated constant
after \(M\) steps of the algorithm. Since \(R^{-1/3}\le R^{-1/9}R^{-\varepsilon ^{2} M/2}\), we have \(M\le \varepsilon ^{-2}/2\). Therefore, taking \(\delta =\varepsilon ^{4}\) gives
which suffices to prove the proposition. □
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Acknowledgements
I am grateful for the mentorship of Larry Guth, with whom I discussed many methods for approaching the moment curve. I also want to thank Ciprian Demeter for helpful conversations about background.
Funding
DM is supported by the National Science Foundation under Award No. 2103249.
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Appendices
Appendix A
1.1 A.1 An \(L^{3/2}\) square function estimate for the parabola
Let \(\mathbb{P}^{1}=\{(t,t^{2}):0\le t\le 1\}\) and for \(r\ge 1\), let \(\mathcal {N}_{r^{-1}}(\mathbb{P}^{1})\) denote the \(r^{-1}\)-neighborhood of \(\mathbb{P}^{1}\) in \(\mathbb{R}^{2}\). Define the collection of canonical \(\sim r^{-1/2}\times r^{-1}\) parabola blocks as follows. Let \(s\in 2^{\mathbb{Z}}\) be the smallest number satisfying \(r^{-1}\le s^{2}\). Then write \(\mathcal {N}_{s^{2}}(\mathbb{P}^{1})\) as
and the two end pieces
We use the notation \(\ell (\tau )=r^{-1/2}\) in two ways: (1) to describe \(\tau \) as one of the sets from the above partition and (2) to index the set of \(\tau \) from the above partition.
Define the \(L^{7/2}\) parabolic square function constant \(\text{PS}(r)\) to be the infimum of \(A>0\) which satisfy
for any Schwartz function \(h:\mathbb{R}^{2}\to \mathbb{C}\) with Fourier transform supported in \(\mathcal {N}_{r^{-1}}(\mathbb{P}^{1})\). Note that \(A\sim (r^{1/2})^{7/4}\) satisfies the displayed inequality for any \(h\), so \(\text{PS}(r)\lesssim r^{7/8}\). The next proposition says that \(\text{PS}(r)\) satisfies a multiscale inequality, which follows from a broad-narrow analysis and bilinear restriction for the parabola.
Proposition 7.1
For each \(1\le L^{2}\le r\),
Proof
Write \(f=\sum _{\ell (\tau )={L^{-1}}}f_{\tau}\). The broad-narrow inequality is
Indeed, suppose that
Let \(\tau _{0}\), \(\ell (\tau _{0})=L^{-1}\) satisfy \(|f_{\tau _{0}}(x)|=\max _{\ell (\tau )=L^{-1}}|f_{\tau}(x)|\). Let \(\ell (\tau _{0}')=4L^{-1}\) contain \(\tau _{0}\) and its neighbors. Then
Then \(|f(x)|^{2}\le (1+\frac{8}{L})|f_{\tau _{0}'}(x)|^{2}\), giving the first term from the upper bound in (47) and finishing the justification for (47).
Suppose that
For each \(\ell (\tau )={4L^{-1}}\), by parabolic rescaling,
The alternative is that
where \(\text{Br}=\{x\in \mathbb{R}^{2}:|h(x)|\le 2L^{3}\max _{ \substack{\ell (\tau )=\ell (\tau ')=L^{-1} \\d(\tau ,\tau ')\ge L^{-1}}}|h_{ \tau}(x)h_{\tau '}(x)|\}\), which we call the broad set. Let \(B_{r^{1/2}}\subset \mathbb{R}^{2}\) be a ball of radius \(r^{1/2}\). Write
where \(B_{r^{1/2}}(\lambda )=\{x\in B_{r^{1/2}}:|h(x)|\sim \lambda \|h\|_{L^{ \infty}(B_{r})}\}\) and \(B_{r^{1/2}}(L)=\{x\in B_{r^{1/2}}:|h(x)|\le r^{-1000}\|h\|_{L^{ \infty}(B_{r^{1/2}})}\}\). Using the locally constant property, note that
Finally, suppose that \(\lambda \in [r^{-1000},1]\) is a dyadic number satisfying
Then we have
and by bilinear restriction for the parabola (see for example Theorem 15 of [FGM21]),
If \(\lambda \|h\|_{L^{\infty}(B_{r^{1/2}})}\le \|\sum _{\theta}|h_{ \theta}|^{2}*w_{r^{1/2}}\|_{L^{\infty}(B_{r^{1/2}})}^{1/2}\), then from (48),
If \(\lambda \|h\|_{L^{\infty}(B_{r^{1/2}})}> \|\sum _{\theta}|h_{\theta}|^{2}*w_{r^{1/2}} \|_{L^{\infty}(B_{r^{1/2}})}^{1/2}\), then using (49), we have
Combined with (48), we have shown that
Summing over \(B_{r^{1/2}}\) in a finitely overlapping cover of \(\mathbb{R}^{2}\) finishes the argument. □
Corollary 7.2
For each \(r\ge 1\),
Proof
Let \(L\) be a constant we allow to depend on \(\delta >0\). If \(1\le r\le L^{2}\), then by Cauchy-Schwarz,
which means that \(\text{PS}(r)\le C_{\delta }\) for all \(r\le L^{2}\) (where \(C_{\delta }\) is permitted to depend on \(\delta \) and \(L\)). Now suppose that \(r>L^{2}\). Let \(m\) satisfy
Then by iterating Proposition 7.1, we have
Since \(16^{m}r/L^{2m}\le L\), we have \(\text{PS}(16^{m}r/L^{2m})\le C_{\delta }\). By definition, \(m\) satisfies \(m\le c\log r/\log L\). Thus the above inequality implies
which finishes the proof by taking \(L\) large enough depending on \(\delta \). □
1.1.1 A.1.1 Proofs of Theorem 4.1 and Corollary 4.2
Recall the statement of Theorem 4.1.
Theorem 1
Cylindrical \(L^{3.5}\) square function estimate over \(\mathbb{P}^{1}\)
Let \(\mathbb{P}^{1}=\{(t,t^{2}):0\le t\le 1\}\) and for \(r\ge 1\), let \(\mathcal {N}_{r^{-1}}(\mathbb{P}^{1})\) denote the \(r^{-1}\)-neighborhood of \(\mathcal {P}^{1}\) in \(\mathbb{R}^{2}\). If \(h:\mathbb{R}^{3}\to \mathbb{C}\) is a Schwartz function with Fourier transform supported in \(\mathcal {N}_{r^{-1}}(\mathbb{P}^{1})\times \mathbb{R}\), then
where the \(\zeta \) are products of approximate rectangles \(\theta \), \(\ell (\theta )={r^{-1/2}}\), with ℝ.
Proof
Begin by using Fourier inversion to write
For each \(x_{3}\), the function \(x'\mapsto \int _{\mathcal {N}_{r^{-1}}(\mathbb{P}^{1})}\int _{\mathbb{R}}\widehat{h}(\xi ', \xi _{3})e^{2\pi i \xi _{3}x_{3}} d\xi _{3}e^{2\pi i \xi \cdot x'}d \xi '\) satisfies the hypotheses of the decoupling theorem for \(\mathbb{P}^{1}\). Use Fubini’s theorem to apply Corollary 7.2 to the inner integral
where the sum in \(\theta \) is over \(\ell (\theta )={r^{-1/2}}\). The sets \(\theta \times \mathbb{R}\) are the \(\zeta \) in the statement of the lemma, so we are done. □
Recall the statement of Corollary 4.2.
Corollary 1
Let \(B_{r}\) be an \(r\)-ball in \(\mathbb{R}^{3}\). If \(h:\mathbb{R}^{3}\to \mathbb{C}\) is a Schwartz function with Fourier transform supported in \(\mathcal {N}_{r^{-1}}(\mathbb{P}^{1})\times \mathbb{R}\), then
where the \(\zeta \) are products of approximate rectangles \(\theta \), \(\ell (\theta )={r^{-1/2}}\), with ℝ.
Proof
Write
Let \(\rho _{r}:\mathbb{R}^{2}\to [0,\infty )\) be a compactly supported smooth function supported in the ball of radius \(r\) centered at the origin. Define \(\phi _{k}:\mathbb{R}^{2}\to [0,\infty )\) by where \(A_{k}=2^{k}B_{r}\setminus 2^{k-1}B_{r}\) and let . Then the right hand side in the previous displayed math is bounded by
We may partition the \(\zeta \) into \(O(1)\) many collections \(\Xi _{i}\) so that the Fourier support of \(h_{\zeta} \varphi _{k}\) is pairwise disjoint for all \(\zeta \in \Xi _{i}\). Finally, by the triangle inequality, for some \(i\), the previous displayed line is bounded by a constant multiple of
which, by Theorem 4.1, is bounded by
Finally, observe that \(\sum _{k=0}^{\infty}\frac{1}{2^{10k}}\varphi _{k}^{7/2}\lesssim W_{B_{r}}\). □
1.2 A.2 An \(\ell ^{7/4}\)-estimate for the cone
Let \(\Gamma =\{(\xi _{1},\xi _{2},\xi _{3})\in \mathbb{R}^{3}:\xi _{1}^{2}+\xi _{2}^{2}= \xi _{3}^{2},\quad \frac{1}{2}\le \xi _{3}\le 1\}\) be the truncated cone. In this section, let \({\mathbf{{S}}}_{r^{-1/2}}\) denote the collection of \(1\times r^{-1/2}\times r^{-1}\) blocks which tile \(\mathcal {N}_{r^{-1}}(\Gamma )\), as defined in §5 of [GM22a].
Recall the statement of Proposition 4.4.
Proposition 1
For any Schwartz function \(h:\mathbb{R}^{3}\to \mathbb{C}\) with \(\widehat{h}\) supported in \(\mathcal {N}_{r^{-1}}(\Gamma )\), we have
It suffices to prove a local version of Proposition 4.4.
Lemma 7.3
Suppose that for any \(r\)-ball \(B_{r}\subset \mathbb{R}^{3}\),
for any Schwartz function \(h:\mathbb{R}^{3}\to \mathbb{C}\) with Fourier transform supported in \(\mathcal {N}_{r^{-1}}(\Gamma )\). Then Proposition 4.4is true.
Proof
Write
where the sum is over a finitely overlapping cover of \(\mathbb{R}^{3}\) by \(r\)-balls. Let \(\phi _{B_{r}}\) be a weight function decaying by order 100 away from \(B_{r}\), satisfying \(\phi _{B_{r}}\gtrsim 1\) on \(B_{r}\), and with Fourier transform supported in an \(R^{-1}\) neighborhood of the origin. For each \(\theta \in{\mathbf{{S}}}_{r^{-1/2}}\), the Fourier support of \(h_{\theta}\phi _{B_{r}}\) is contained in a \(1\times 2r^{-1/2}\times 2r^{-1}\) conical block. By the triangle inequality, there is a subset \(\mathcal {S}\) of the cone blocks \(\theta \) so that for each \(\theta \in \mathcal {S}\), the Fourier support of \(f_{\theta}\phi _{B_{r}}\) is contained in a unique cone block and
Then by applying the hypothesized local version of Proposition 4.4,
It remains to note that
□
It suffices to prove a weak, level-set version of Proposition 4.4.
Lemma 7.4
For each \(B_{r}\) and Schwartz function \(h:\mathbb{R}^{3}\to \mathbb{C}\) with Fourier transform supported in \(\mathcal {N}_{r^{-1}}(\Gamma )\), there exists \(\alpha >0\) such that
Proof
By an analogous proof as for Lemma 7.4 for the cone, the argument reduces to bounding
By Hölder’s inequality, we have
Finally, by the locally constant property and Hölder’s inequality,
where we note that for \(U\|U_{\theta ,r}\), \(|U|=|\theta ^{*}|\). □
Use the notation
We will show that to estimate the size of \(U_{\underline {\alpha }}\), it suffices to replace \(h\) with a version whose wave packets have been pigeonholed. Write
where for each \(\theta \), \(\{\psi _{T}\}_{T\in \mathbb{T}_{\theta}}\) is analogous to the partition of unity from §2.1, but adapted to \(\theta ^{*}\), the dual sets of conical blocks \(\theta \). If \(\underline {\alpha }\le C_{\varepsilon }(\log r)r^{-500}\max _{\theta}\|h_{\theta} \|_{\infty}\), then by an analogous argument as dealing with the low integral over \(\{x:|h(x)|\le r^{-1000}\|h\|_{L^{\infty}(B_{r})}\}\) in the proof of Lemma 7.4, bounding \(\underline {\alpha }^{7/2}|U_{\underline {\alpha }}|\) by the right hand side of Proposition 4.4 is trivial. Let \(\phi _{B_{r}}\) be the weight function from Lemma 7.3.
Proposition 7.5
Wave packet decomposition
Let \(\underline {\alpha }>C_{\varepsilon }(\log r) r^{-100}\times \max _{\theta}\|h_{\theta}\|_{L^{ \infty}(\mathbb{R}^{3})}\). There exist subsets \(\mathcal {S}\subset{\mathbf{{S}}}_{r^{-1/2}}\) and \(\tilde{\mathbb{T}}_{\theta}\subset \mathbb{T}_{\theta}\), as well as a constant \(A>0\) with the following properties:
The justification for this proposition follows an analogous argument as for Proposition 6.4, so we omit the proof.
Proof of Proposition 4.4
By Lemma 7.3, Lemma 7.4, and Proposition 7.5, it suffices to show that for some \(\underline {\alpha }\ge C_{\varepsilon }r^{-100}\max _{\theta \in{\mathbf{{S}}}_{r^{-1/2}}} \|h_{\theta}\|_{L^{\infty}(\mathbb{R}^{3})}\),
where
and \(\mathcal {S}\subset{\mathbf{{S}}}_{r^{-1/2}}\) and \(\tilde{\mathbb{T}}_{\theta}\) are from the proof of Proposition 7.5. The wave envelope estimate (Theorem 1.3 from [GWZ20]) gives the inequality
The inequality (55) follows from the above inequality if
Suppose that this is not the case. By Proposition 7.5 and the assumption that \(\underline {\alpha }\ge C_{\varepsilon }r^{-100} \max _{\theta}\|h_{\theta}\|_{L^{ \infty}(\mathbb{R}^{3})}\) is bounded below, we have the set inclusion \(U_{\underline {\alpha }}'\subset \cup _{\theta \in \mathcal {S}}\cup _{T\in \tilde{\mathbb{T}}_{\theta}}r^{\varepsilon }T\). Using this with the assumption that (56) does not hold, we have
where we also used (53) and (54) from Proposition 7.5. Then using the locally constant property and Hölder’s inequality, we have
We are done after noting that \(|T|=|\theta ^{*}|\) and \(T\in \tilde{\mathbb{T}}_{\theta}\) is a subset of \(U\|U_{\theta ,r}\). □
Appendix B
We sketch the adaptation of Theorem 1 to general curves \(\gamma \) with torsion. Let \(\gamma :[0,1]\to \mathbb{R}^{3}\) be a \(C^{4}\) curve satisfying
For each \(R\in 8^{\mathbb{N}}\), define the anisotropic neighborhood
Partition the neighborhood into blocks \(\theta \in{\mathbf{{S}}}_{\gamma }(R^{-1/3})\) of the form
where \(B\) and \(C\) are ℝ-valued parameters and \(l\in \{0,\ldots ,R^{1/3}-1\}\). The general version of Theorem 1 is the following.
Theorem 8.1
Let \(\gamma \) satisfy (57). For any \(\varepsilon >0\), there exists \(C_{\varepsilon }<\infty \) such that
For any Schwartz function \(f:\mathbb{R}^{3}\to \mathbb{C}\) with Fourier transform supported in \(\mathcal {M}_{\gamma }^{3}(R)\).
We note that the condition that \(\gamma \) is \(C^{4}\) may be relaxed to \(C^{3}\) if we describe how to carry out each step of the proof of Theorem 1 adapted to \(\gamma \). By assuming that \(\gamma \) is \(C^{4}\), we may use a vastly simpler argument involving Taylor approximation and resembling the iteration in the proof of Proposition 6.8. The constant \(C_{\varepsilon }\) in (58) is permitted to depend on \(\varepsilon \) and on \(\gamma \). To prove Theorem 8.1, we will adapt the proof of Theorem 1 to hold for a specialized class \(\mathcal {C}\) of curves \(\gamma \) which is closed under certain affine rescalings. The \(C_{\varepsilon }\) constant will be uniform for \(\gamma \) in the class \(\mathcal {C}\).
Let \(\frac{1}{2}\ge a>0\) and \(\frac{a}{4}\ge \nu >0\). Define the class \({\mathcal {C}}\) to be the collection of \(C^{3}\) curves \(\gamma :[0,1]\to \mathbb{R}^{3}\) satisfying
By the inverse function theorem and by possible interchanging the roles of \(\gamma _{2}\) and \(\gamma _{3}\), it is always possible to divide a general \(\gamma \) satisfying (57) into sub-pieces \(\left .\gamma \right |_{[c,c+\varepsilon _{0}]}\) (for some \(\varepsilon _{0}>0\) depending on \(\gamma \)), each of which may be reparameterized so that it is contained in \(\mathcal {C}\) for some \(\nu ,a\). Then (58) will hold with a factor of \(\varepsilon _{0}^{-1}\) times the maximum of the \(C_{\varepsilon }\) which work for each sub-piece of \(\gamma \).
For each \(R\ge 1\), let \(S(R)\) denote the smallest constant so that
where \(f:\mathbb{R}^{3}\to \mathbb{C}\) is a Schwartz function with \(\mathrm {supp}\widehat{f}\subset \mathcal {M}^{3}_{\gamma }(R)\) and \(\gamma \) is any curve in \(\mathcal {C}\).
Proof of Theorem 8.1
Our goal is to show that \(S(R)\lesssim _{\varepsilon }R^{\varepsilon }\). By possibly replacing \(S(R)\) by \(\sup _{1\le r\le R}S(r)\), it is no loss of generality to assume that \(S(R)\) is a nondecreasing function of \(R\). Let \(\varepsilon >0\). Let \(\gamma \in \mathcal {C}\) and let \(f:\mathbb{R}^{3}\to \mathbb{C}\) be a Schwartz function with Fourier transform supported in \(\mathcal {M}^{3}_{\gamma }(R)\). Write \(K>0\) for a parameter we will choose to be a small power of \(R\) later in the proof. We will show the multiscale inequality that for any \(\delta _{1},\delta _{2}>0\),
The bound \(S(R)\lesssim _{\varepsilon }R^{\varepsilon }\) then follows via an analogous argument as the proof of Theorem 1 from Proposition 6.8. To prove the multiscale inequality, we use a simpler version of the argument from Proposition 6.8, highlighting steps which are different. Begin with the defining inequality for \(S(R/K)\):
The square function we are aiming for is \(\sum _{\theta \in{\mathbf{{S}}}_{\gamma }(R^{-1/3})}|f_{\theta}|^{2}\). Assume that
As in the proof of Proposition 6.8, if this does not hold, then
and we have shown that \(S(R)\lesssim S(R/K)\) in this case.
Next we describe an iterative procedure. The initial step is special, so we describe the first two steps and, if the process does not already terminate, iterate the second step. The Fourier support of is in an annulus \(\{R^{1/3}\lesssim |\xi |\lesssim (R/K)^{-1/3}\}\). Let \(s_{1}\) be a dyadic value in the range \(R^{-1/3}\lesssim s_{1}\lesssim (R/K)^{-1/3}\) satisfying
Then by pointwise local \(L^{2}\)-orthogonality,
where \(\tau '\sim \tau ''\) means \(d(\tau ',\tau '')\lesssim s_{1}\). For each \(\tau \in{\mathbf{{S}}}_{\gamma }((R/K)^{-1/3})\) and \(\tau '\subset \tau \), \(\tau '\in{\mathbf{{S}}}_{\gamma }(s_{1})\), the Fourier support of
is contained in \((10\tau '-10\tau ')\setminus B_{s_{1}}\), which, after dilating by a factor of \(s_{1}^{-1}\), we may identify with a conical cap as we did in §3. Therefore, we may apply a version of Proposition 4.4 uniform for \(\gamma \in \mathcal {C}\) (see §B.5 for the adaptation to general \(\gamma \)) to obtain
For each \(s_{1}\le \sigma \le 1\), \(\underline {\tau}\in{\mathbf{{S}}}_{\gamma }(\sigma ^{-1}s_{1})\), and \(V\|V_{\underline {\tau},s_{1}^{-3}}^{\gamma }\), by Cauchy-Schwarz, Hölder’s inequality, and properties of weight functions (using that \(B_{s_{1}}(0)\subset V_{\tau ,s_{1}^{-3}}^{\gamma }\)),
Suppose a certain \(\sigma \) term dominates, so that (65) is bounded by
If \(\sigma < K^{-\varepsilon }\), then use a general Corollary 4.2, Cauchy-Schwarz, and Hölder’s inequality to bound the above expression by
The other case is that \(\sigma \ge K^{-\varepsilon }\). Then (66) is bounded by
By Taylor approximation, the Fourier support of \(f_{\tau}\) is contained in the \(C(R/K)^{-4/3}\)-neighborhood of
Assume that \((R/K)^{-4/3}\le R^{-1}\). Then after an affine transformation with determinant uniform over \(\mathcal {C}\) (see §B.3), this is a subset of \(\mathcal {M}^{3}(R)\), the anisotropic neighborhood of the moment curve. Therefore, by Theorem 1,
Since \(\|\cdot \|_{\ell ^{7/2}}\le \|\cdot \|_{\ell ^{1}}\), the right hand side is bounded by
The iteration terminates with the conclusion that \(S(R)\le C_{\delta }(\log R)R^{2\delta }K^{\varepsilon }S(R/K)\) in this case.
Assume from now that \(\sigma < K^{-\varepsilon }\) and the outcome of the first step was
We may now repeat the argument laid out so far but with \(\sum _{\tau ''\in{\mathbf{{S}}}_{\gamma }(K^{-\varepsilon /2}s_{1})}|f_{\tau ''}|^{2}\) in place of \(\sum _{\tau \in{\mathbf{{S}}}_{\gamma }((R/K)^{-1/3})}|f_{\tau}|^{2}\). After \(m\) iterations, conclude that
in which \(s_{m}\le K^{-m\varepsilon /2}(R/K)^{-1/3}\). The algorithm terminates in at most \(M\) steps where \(K^{-M\varepsilon /2}(R/K)^{-1/3}\sim R^{-1/3}\), so \(M\sim \varepsilon ^{-1}\). The conclusion is then
recalling the condition from earlier that \(K\le R^{1/4}\). If for \(\eta >0\), \(\sup _{R\ge 1}S(R)\lesssim _{\eta }R^{\eta}\), then we also have that for each \(R\gtrsim _{\varepsilon }1\),
where we are free to choose \(\delta >0\), \(\varepsilon >0\), and \(K\le R^{1/4}\). Letting \(\delta =\varepsilon ^{3}\), \(\varepsilon =\eta /2\), and \(K=R^{\varepsilon }\), we see that the above inequality implies
This means that the infimum of \(\eta >0\) such that \(\sup _{R\ge 1}S(R)\lesssim _{\eta }R^{\eta}\) is zero, as desired. □
2.1 B.3 Affine rescaling for \(\gamma \in \mathcal {C}\)
Recall the definition of \(\mathcal {C}\). Let \(\frac{1}{2}\ge a>0\) and \(\frac{a}{4}\ge \nu >0\). The class \({\mathcal {C}}\) is the collection of \(C^{4}\) curves \(\gamma :[0,1]\to \mathbb{R}^{3}\) satisfying
Let \(C_{0}>0\) to be a constant that is permitted to depend on \(a\) and \(\nu \). Consider \(C_{0}\le S< R\) and \(\tau \in{\mathbf{{S}}}_{\gamma }(S^{-1/3})\). We will show that there exists \(\tilde{\gamma }\in \mathcal {C}\) and an affine transformation \(A_{\tau}: \mathbb{R}^{3}\to \mathbb{R}^{3}\) mapping \(\tau \) to \([0,1]^{3}\) and mapping each \(\theta \in{\mathbf{{S}}}_{\gamma }(R^{-1/3})\) with \(\theta \subset \tau \) to \(A(\theta )\in{\mathbf{{S}}}_{\tilde{\gamma }}((R/S)^{-1/3})\). Suppose that \(\tau \) is the \(l\)th piece in \({\mathbf{{S}}}(S^{-1/3})\) so that
Let \(t_{0}=lS^{-1/3}\) and define \(A_{\tau}\) to be the map
in which \(c_{\tau}= \frac{{\gamma }''(t_{0})}{2[\gamma _{2}''(t_{0})\gamma _{3}'''(t_{0})-\gamma _{3}''(t_{0})\gamma _{2}'''(t_{0})]}\). Define \(s=S^{1/3}(t-t_{0})\). For \(0\le s\le 1\), let \(\tilde{\gamma }(s)= A_{\tau} \gamma (t)\) so that we may write \(\tilde{\gamma }(s)=(s,\tilde{\gamma }_{2}(s),\tilde{\gamma }_{3}(s))\), where
We now verify that \(\tilde{\gamma }\in \mathcal {C}\). Clearly, \(\tilde{\gamma }\) is \(C^{4}\) and has the form (67). Since \(\|\gamma _{2}\|_{C^{4}}\le 1\), it is straightforward to verify that \(\|\tilde{\gamma }_{2}\|_{C^{4}}\le 1\). Since \(\|\gamma _{3}\|_{C^{4}}\le 1\), \(\|\tilde{\gamma }_{2}\|_{C^{4}}\le 1\), and \(S\) is sufficiently large depending on \(a\) and \(\nu \), it is then easy to check that \(\|\tilde{\gamma }_{3}\|_{C^{4}}\le 1\), which verifies (69). Note the form of the following derivatives
Clearly \(\gamma _{2}''(t)\ge a\) implies that \(\tilde{\gamma }_{2}''(s)\ge a\). By Taylor approximation, the above expression shows that \(\tilde{\gamma }_{3}'''(s)=1+O(S^{-1/3})\). Since \(a\le 1/2\) and \(S\) is at least a certain size depending on \(a\) and \(\nu \), we have that \(\tilde{\gamma }_{3}'''(s)\ge a\), which verifies (68). Using similar reasoning, it is straightforward to check (69). Finally, we have
where we used Taylor approximation in the final inequality. Since we assumed that \(\nu <\frac{a}{4}\) and \(S\) is large depending on \(a\) and \(\nu \), property (70) holds. This concludes the verification that \(\tilde{\gamma }\in \mathcal {C}\). We record this in the following lemma.
Lemma 8.2
General affine rescaling
Let \(C_{0}\) be a sufficiently large constant depending on \(\nu \) and \(a\). Let \(C_{0}\le S\le R\) and \(\tau \in{\mathbf{{S}}}_{\gamma }(S^{-1/3})\). There exists \(\tilde{\gamma }\in \mathcal {C}\) such that for each \(\theta \in{\mathbf{{S}}}_{\gamma }(R^{-1/3})\), \(A_{\tau}\theta \in{\mathbf{{S}}}_{\tilde{\gamma }}((R/S)^{-1/3})\).
Proof
From the discussion preceding the lemma, it remains to check how \(A_{\tau}\) transforms the blocks \(\theta \in{\mathbf{{S}}}_{\gamma }(R^{-1/3})\). For \(m\in \{0,\ldots ,R^{1/3}-1\}\) with \(lS^{-1/3}\le mR^{-1/3}<(l+1)S^{-1/3}\), consider
Applying \(A_{\tau}\) yields
which is clearly an element of \({\mathbf{{S}}}_{\tilde{\gamma }}((R/S)^{-1/3})\). □
2.2 B.4 The general versions of Theorem 4.1 and Corollary 4.2
We claim that for each \(\gamma \in \mathcal {C}\), Theorem 4.1 and Corollary 4.2 hold with \((t,\gamma _{2}(t))\) in place of the parabola \((t,t^{2})\). We following the argument from §A.1. First define \(\text{PS}_{\gamma }(r)\) to be the analogue of \(\text{PS}(r)\) for each \(\gamma \in \mathcal {C}\). Then let \(\text{PS}_{\mathcal {C}}(r)=\sup _{\gamma \in \mathcal {C}}\text{PS}_{\gamma }(r)\). The quantity \(\text{PS}_{\mathcal {C}}(r)\) satisfies an analogous multiscale inequality as \(\text{PS}(r)\) does in Proposition 7.1. In the narrow case of the proof of Proposition 7.1, we have
in which \(h:\mathbb{R}^{2}\to \mathbb{C}\) is a Schwartz function with Fourier support in \(\mathcal {N}_{r^{-1}}(\{(t,\gamma _{2}(t)):0\le t\le 1\})\) and \(\tau \) are approximate rectangles of the form
Instead of invoking parabolic rescaling, we rescale the Fourier side using the affine map \(B_{\tau}: \mathbb{R}^{2}\to \mathbb{R}^{2}\) defined by
The map \(B_{\tau}\) takes each \(\theta \) block of \((t,\gamma _{2}(t))\) of dimensions \(\sim r^{-1/2}\times r^{-1}\) to a block of \((t,\tilde{\gamma }_{2}(t))\) with dimensions \(\sim (4r/L)^{-1/2}\times (4r/L)\), where \(\tilde{\gamma }\) is the same curve defined in §B.3. This allows us to conclude that
as we did in the parabola case. The final adaptation in the proof of Proposition 7.1 is to note that the bilinear restriction estimate that is referenced also holds uniformly for \(\gamma \in \mathcal {C}\), which is clear from the proof of Theorem 15 in [FGM21].
Concluding that \(\text{PS}_{\mathcal {C}}(r)\lesssim _{\varepsilon }r^{\varepsilon }\) after proving the multiscale inequality follows from the same argument as for the parabola. With the boundedness of \(\text{PS}_{\mathcal {C}}(r)\), the proofs of Theorem 4.1 and Corollary 4.2 for \((t,\gamma _{2}(t))\) in place of \((t,t^{2})\) are unchanged.
2.3 B.5 The general version of Proposition 4.4
In this section, we describe how to obtain a version of Proposition 4.4 that holds uniformly for the general cones that arise from analyzing \(\gamma \in \mathcal {C}\). The argument proving Proposition 4.4 adapts immediately to those cones, except that we must invoke a general version of the \(L^{4}\) wave envelope estimate Theorem 1.3 from [GWZ20] (which was proven for the light cone). It therefore suffices to prove a certain generalization of Theorem 1.3 from [GWZ20].
Before stating the theorem we need to prove, we present an abbreviated version of §3 which describes the geometric relationship between moment curve blocks and cone planks. When we describe sets as comparable or use \(O(\cdot )\) notation, we shall always mean up to constants which are permitted to depend on \(\nu \) and \(a\) from the definition of \(\mathcal {C}\). Let \(\gamma \in \mathcal {C}\) and consider \(\theta \in{\mathbf{{S}}}_{\gamma }(R^{-1/3})\) given by
where \(l\) is some integer in the range \(0\le l\le R^{1/3}-1\). Up to a \(O(R^{-1})\) error, the above set is approximately
The Fourier support of \(\sum _{\theta \in{\mathbf{{S}}}_{\gamma }(R^{-1/3})}|f_{\theta}|^{2}\) is contained in the union \(\cup _{\theta \in{\mathbf{{S}}}_{\gamma }(R^{-1/3})}(\theta -\theta )\). The sets \(\theta -\theta \) are
Furthermore, on the annulus \(|\xi |\sim R^{-1/3}\), \(\theta -\theta \) is comparable to
The right hand side is an \(R^{-1/3}\)-dilation of the \(R^{-2/3}\)-neighborhood of a plank from the generalized cone
For \(S\ge 1\), let \({\mathbf{{T}}}_{\gamma }(S^{-1/2})\) denote a collection of finitely overlapping planks \(\zeta \) with dimensions \(\sim 1\times S^{-1/2}\times S^{-1}\) whose union is approximately the \(S^{-1}\) neighborhood of \(\Gamma _{\gamma }\). Each \(\zeta \in{\mathbf{{T}}}_{\gamma }(S^{-1/2})\) is comparable to the \(S^{-1}\) neighborhood of a sector
For each \(\zeta \in{\mathbf{{S}}}_{\gamma }(S^{-1/2})\), let \(\zeta ^{*}\) be a parallelogram with right angles that is dual to \(\zeta \), centered at the origin, and has dimensions \(\sim 1\times S^{1/2}\times S\). For each dyadic \(\sigma \in [S^{-1/2},1]\) and each \(\tau \in{\mathbf{{T}}}_{\gamma }(\sigma ^{-1}S^{-1/2})\), let \(U_{\tau ,S}\) denote an anisotropically dilated version of \(\tau ^{*}\) which is comparable to
The wave envelope \(U_{\tau ,S}\) has dimensions \(\sim \sigma ^{-2}\times \sigma ^{-1}S^{1/2}\times S\). Write \(U\|U_{\tau ,S}\) for a tiling of \(\mathbb{R}^{3}\) by translates of \(U_{\tau ,S}\). Now we may state the theorems we must prove for our general cones. A general \(L^{4}\) wave envelope estimate for \(\Gamma _{\gamma }\) (the analogue of Theorem 1.3 from [GWZ20]) follows from the following two theorems.
Theorem 2
For each \(\varepsilon >0\), there exists \(C_{\varepsilon }<\infty \) such that the following holds. For any \(S\in 4^{\mathbb{N}}\) and \(\gamma \in \mathcal {C}\), if \(f:\mathbb{R}^{3}\to \mathbb{C}\) is a Schwartz function with \(\mathrm {supp}\widehat{f}\subset \mathcal {N}_{S^{-1}}(\Gamma _{\gamma })\), then
Theorem 3
For each \(\varepsilon >0\), there exists \(C_{\varepsilon }<\infty \) such that the following holds. For any \(S\in 4^{\mathbb{N}}\) and \(\gamma \in \mathcal {C}\), if \(f:\mathbb{R}^{3}\to \mathbb{C}\) is a Schwartz function with \(\mathrm {supp}\widehat{f}\subset \mathcal {N}_{S^{-1}}(\Gamma _{\gamma })\), then
First we prove Theorem 2 assuming Theorem 3.
Proof of Theorem 2
Let \(T(S)\) be the infimum of constants \(A>0\) such that
for any Schwartz function \(f\) with Fourier support in \(\mathcal {N}_{S^{-1}}(\Gamma _{\gamma })\), for any \(\gamma \in \mathcal {C}\). Let \(K< S\) be a large parameter we will specify later. Fix a Schwartz \(f:\mathbb{R}^{3}\to \mathbb{C}\) with Fourier transform supported in \(\mathcal {N}_{S^{-1}}(\Gamma _{\gamma })\), for some \(\gamma \in \mathcal {C}\). Using the definition of \(T(\cdot )\), we have
in which the \(\zeta _{0}\) vary over the set \({\mathbf{{T}}}_{\gamma }((S/K)^{-1/2})\). Apply Theorem 3 to obtain
If \(\sigma ^{-2}>S^{1/2}\), then using local \(L^{2}\) orthogonality, we have
where the \(\zeta \) are in \({\mathbf{{T}}}_{\gamma }(S^{-1/2})\). Then by Cauchy-Schwarz and \(\|\cdot \|_{\ell ^{2}}\le \|\cdot \|_{\ell ^{1}}\), the right hand side above is bounded by a constant times \(\int |\sum _{\zeta }|f_{\zeta }|^{2}|^{2}\).
Now suppose that \(\sigma ^{-2}\le S^{1/2}\). Consider \(\tau \in{\mathbf{{T}}}_{\gamma }(\sigma ^{-1}S^{-1/2})\) which is a neighborhood of the sector
Write \(r=\sigma S^{1/2}\). The affine transformation \(B_{\tau}: \mathbb{R}^{3}\to \mathbb{R}^{3}\) defined by
maps \(X_{\tau}\) to \(\Gamma _{\tilde{\gamma }}\), where \(\tilde{\gamma }\in \mathcal {C}\) is the same curve that \(\gamma \) maps to after using the affine transformation from §B.3. Note that
Rescaling the Fourier side using \(B_{\tau}\) and using the definition of \(T(\cdot )\) again, we may use Khintchin’s inequality to select \(c_{\zeta _{0}}\in \{\pm 1\}\) satisfying
Conclude from this argument that
Choose \(K=S^{3/4}\) and assume without loss of generality that \(S(\cdot )\) is a nondecreasing function so that the above inequality implies that \(T(S)\lesssim _{\delta }S^{\delta }T(S^{1/4})T(S^{5/8})\). Since \(\delta >0\) is arbitrarily small, conclude that the infimum of \(\eta >0\) such that \(\sup _{S\ge 1}T(S)\lesssim _{\eta }S^{\eta}\) must be zero. □
Now we prove Theorem 3, which is a succinct version of the proof of Lemma 1.4 in [GWZ20].
Proof of Theorem 3
Fix \(\gamma \in \mathcal {C}\) and a Schwartz \(f:\mathbb{R}^{3}\to \mathbb{C}\) with \(\mathrm {supp}\widehat{f}\subset \mathcal {N}_{S^{-1}}(\Gamma _{\gamma })\). By Plancherel’s theorem, we have
The Fourier transforms \(\widehat{|f_{\zeta }|^{2}}\) are supported in \(\zeta -\zeta \), which is essentially \(\zeta \) translated to the origin. For each dyadic \(\sigma \), \(S^{-1/2}< \sigma \lesssim 1\) and each \(\zeta \in{\mathbf{{T}}}_{\gamma }(S^{-1/2})\), define
For \(\sigma =S^{-1/2}\), define \(\zeta _{S^{-1/2}}\) to be
Note that \(\zeta -\zeta \) is contained in \(\cup _{\sigma }\zeta _{\sigma}\). Write \(\Omega _{\sigma}=\cup _{\zeta }\zeta _{\sigma}\). Suppose that
First we will show that
The above inequality is permitted to have implicit constants depending on the parameters \(a,\nu \) from the definition of \(\mathcal {C}\). Therefore, it suffices to show that for \(\delta =\delta (a,\nu )>0\) that we will choose later, for each \(\tau '\in{\mathbf{{S}}}_{\gamma }(\delta )\), we have
Consider the intersection \(\Omega _{\sigma}\cap \{\xi \in \mathbb{R}^{3}:\xi _{1}=h\}\) where \(h\ge 0\) (the \(h<0\) case is analogous). Suppose first that \(h\gg \sigma S^{-1/2}\). If \(\{\xi :\xi _{1}=h\}\cap \zeta _{\sigma}\cap \zeta _{\sigma}'\) is nonempty, then since \(\ddot{\gamma }\) has 0 in the first component, there is some choice of parameters \(B,B'\) with \(|B|,|B'|\lesssim \sigma S^{-1/2}\) such that
where \(\zeta \) is the \(l\)th plank and \(\zeta '\) is the \((l')\)th plank. It follows from Taylor’s theorem and the definition of \(\mathcal {C}\) that \(|lS^{-1/2}-l'S^{-1/2}|\lesssim \sigma ^{-1}S^{-1/2}\), so \(\zeta _{\sigma}, \zeta \sigma '\) are contained in the same \(\tau \in{\mathbf{{S}}}_{\gamma }(\sigma ^{-1}S^{-1/2})\).
Similarly, if \(h\ll \sigma S^{-1/2}\), then for some parameters \(B,B'\) with \(|B|\sim |B'|\sim \sigma S^{-1/2}\), (74) holds. In this case, the left hand side is dominated by the difference in the \(\ddot{\gamma }\) terms, which is bounded below by \(\sim |B||lS^{-1/2}-l'S^{-1/2}|\). Conclude again that \(\zeta _{\sigma}\) and \(\zeta _{\sigma '}\) are contained in the same \(\tau \in{\mathbf{{S}}}_{\gamma }(\sigma ^{-1}S^{-1/2})\).
It remains to analyze the case in which \(h\sim \sigma S^{-1/2}\sim |B|\). Fix a \(\tau '\in{\mathbf{{S}}}_{\gamma }(\delta )\). The set \((\cup _{\zeta \subset \tau '}\zeta _{\sigma})\cap \{\xi :\xi _{1}=h\}\) is contained in an \(\sim S^{-1}\)-neighborhood of
where \(I\) is the \(\delta \) interval corresponding to the sector defining \(\tau '\). Fix \(B\) satisfying \(|B|\sim \sigma S^{-1/2}\) and \(t\in I\). Consider the property that \(h\dot{\gamma }(t)+B\ddot{\gamma }(t)\in \mathcal {N}_{S^{-1}}(\zeta _{\sigma})\), where \(\zeta _{\sigma}\) has corresponding parameter \(lS^{-1/2}\in I\). Letting \(t_{k}=k\sigma ^{-1}S^{-1/2}\), \(t_{k}\in I\), we note that if \(|lS^{-1/2}-t_{k}|\le \sigma ^{-1}S^{-1/2}\), then
for any \(B'\) with \(|B'|\sim \sigma S^{-1/2}\). Therefore, to bound the number of \(\zeta _{\sigma}\) within \(\sim S^{-1}\) of \(h\dot{\gamma }(t)+B\ddot{\gamma }(t)\), it suffices to bound the number of \(t_{k}\) for which there exists \(B_{k}\) with \(|B_{k}|\sim \sigma S^{-1/2}\) satisfying
This is because for each \(t_{k}\) satisfying the above inequality, there are \(\sim \sigma ^{-1}\) many \(lS^{-1/2}\) within \(\sigma ^{-1}S^{-1/2}\) of \(t_{k}\) that satisfy a similar inequality. Dividing the previous displayed inequality through by \(h\), we obtain
This implies that
Let \(F_{t}:I\to \mathbb{R}\) be defined by
Note that \(F_{t}(t)=0\), \(F_{t}'(s)=[\dot{\gamma }(t)+\frac{B}{h}\ddot{\gamma }(t)]\cdot (\dot{\gamma }(s) \times \dddot{\gamma }(s))\), \(|F_{t}'(t)|\gtrsim \nu >0\), \(F_{t}''(s)=[\dot{\gamma }(t)+\frac{B}{h}\ddot{\gamma }(t)]\cdot (\dot{\gamma }(s) \times{ \gamma }^{(4)}(s)+\ddot{\gamma }(s)\times \dddot{\gamma }(s))\), and \(|F_{t}''(s)|\lesssim 1\). It follows that for \(\delta \) (the length of the domain interval \(I\)) sufficiently small, depending on \(\nu \), \(|F_{t}(s)|\sim |t-s|\). Conclude that (76) implies that \(|t-t_{k}|\lesssim \sigma ^{-1}S^{-1/2}\). Since the \(t_{k}\) are \(\sigma ^{-1}S^{-1/2}\)-separated, there are \(\lesssim 1\) many \(t_{k}\) which satisfy (76). This finishes the justification of (73).
It remains to bound the integral
for each \(\tau \in{\mathbf{{S}}}_{\gamma }(\sigma ^{-1}S^{-1/2})\). The inequality (75) shows that if \(\zeta \subset \tau \) (\(\tau \) with corresponding parameter \(t_{k}\)), then \(\zeta _{\sigma}\subset C(\zeta _{k})_{\sigma}\), where \(\zeta _{k}\in{\mathbf{{S}}}_{\gamma }(S^{-1/2})\) has parameter \(lS^{-1/2}=t_{k}\). Let \(\eta _{k}\) be a bump function equal to 1 on \(C(\zeta _{k})_{\sigma}\) and with Fourier transform decaying rapidly away from \(U_{\tau ,S}^{*}\), the wave envelope centered at the origin. Then by Cauchy-Schwarz and the decay of , we have
which is the desired upper bound. □
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Maldague, D. A sharp square function estimate for the moment curve in \(\mathbb{R}^{3}\). Invent. math. 238, 175–246 (2024). https://doi.org/10.1007/s00222-024-01282-0
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DOI: https://doi.org/10.1007/s00222-024-01282-0