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An L³ bound for the dyadic triangular Hilbert form
expertly designed by an internal OpenAI model · released 2026-10-05
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IntroductionThe triangular Hilbert form couples three functions of two variables, each pair sharing one variable. We study its dyadic model, in which the intervals are constrained by binary addition without carries. The estimate below imposes no structural condition on any of the three inputs. Write \(\mathbb R_+=[0,\infty)\). For \(k\in\mathbb Z\), let \[\mathcal D_k=\{[2^kn,2^k(n+1)):n\in\mathbb Z_{\ge0}\}.\] For \(I\in\mathcal D_k\), denote its index by \(n_I\) and set \[h_I=\mathbf1_{I_{\mathrm{left}}}-\mathbf1_{I_{\mathrm{right}}}.\] Let \(\oplus\) denote bitwise XOR of nonnegative integers, and define the set of admissible triples \[\mathcal A_k=\{(I_0,I_1,I_2)\in\mathcal D_k^3: n_{I_0}\oplus n_{I_1}\oplus n_{I_2}=0\}.\] For \(\mathbf I\in\mathcal A_k\) and three real functions \(F_v\) on \(\mathbb R_+^2\), put \[ L_{\mathbf I}(F_0,F_1,F_2) =2^{-k}\int_{I_0\times I_1\times I_2} F_0(x_0,x_1)F_1(x_1,x_2)F_2(x_2,x_0) \prod_{v=0}^2 h_{I_v}(x_v)\,\mathrm dx_0\,\mathrm dx_1\,\mathrm dx_2. \tag{1}\] The dyadic triangular Hilbert form with a finite set of scales \(S\subset\mathbb Z\) and real coefficients \(\lvert \epsilon_k\rvert\le1\) is \[ \Lambda^{\mathrm d}_{S,\epsilon}(F_0,F_1,F_2) =\sum_{k\in S}\epsilon_k\sum_{\mathbf I\in\mathcal A_k} L_{\mathbf I}(F_0,F_1,F_2). \tag{2}\] Theorem 1. For every finite \(S\subset\mathbb Z\) and all real bounded compactly supported measurable functions \(F_0,F_1,F_2\) on \(\mathbb R_+^2\), \[ \sum_{k\in S}\sum_{\mathbf I\in\mathcal A_k} \lvert L_{\mathbf I}(F_0,F_1,F_2)\rvert \le 40\prod_{v=0}^2\lVert F_v\rVert_{L^3(\mathbb R_+^2)}. \tag{3}\] In particular, (2) satisfies the same product bound, uniformly in the scales and coefficients. The absolute values in (3) also allow a separate coefficient of modulus at most one for each admissible triple. The estimate extends to all real \(L^3\) inputs by density, as explained in Section 5. Context and relation to earlier workThe continuous triangular Hilbert form has the same cyclic arrangement of inputs as (1), integrated over \(\mathbb R^3\) against the principal-value kernel \(1/(x_0+x_1+x_2)\). Its symmetric \(L^3\) estimate is formulated by Thiele in (Grafakos et al. 2017, sec. 9, Problem 13). That contribution also displays the precise dyadic model (2), with one coefficient for each scale, and asks for the analogous bound. Theorem 1 answers this dyadic question affirmatively and gives the stronger sum of absolute local contributions. The continuous form and its dyadic model are distinct operators; the theorem here is a statement about the latter. Kovač, Thiele and Zorin-Kranich introduced a dyadic triangular model with coefficients allowed to vary among interval triples (Kovač et al. 2015, Equations (1.5)–(1.6)). Their Theorem 1.7 gives uniform estimates when one input has either a specified dependence on a Walsh linear combination of its coordinates or a specified fiberwise character structure. Those cases already encompass dyadic versions of Carleson’s operator and uniform bounds for the bilinear Hilbert transform, as explained in their Appendix A. Our estimate allows all three inputs to vary freely. The cyclic operator-trace representation used below also appears in their Equation (1.5). Another line of work measures cancellation through the growth of truncated norms. Tao obtained sublogarithmic growth for one-dimensional multilinear Hilbert transforms (Tao 2016, Theorem 1.2); Zorin-Kranich proved the corresponding sublinear growth in the number of smooth scales for simplex Hilbert transforms (Zorin-Kranich 2017, Theorem 1.3). Durcik, Kovač and Thiele then obtained power-type cancellation in both the continuous and dyadic settings (Durcik et al. 2019, Theorems 1 and 4). For the triangular dyadic form, their bound over \(m\) consecutive scales has a factor \(m^{1/2}\) at exponents \((4,4,2)\); cyclic permutation and multilinear interpolation give the same growth at \((3,3,3)\). Theorem 1 removes this scale dependence at the symmetric tuple. The strategy of controlling an entangled form by the change of a nonnegative energy has precedents in Kovač’s Bellman-function framework (Kovač 2011, sec. 2) and his telescoping identity for the twisted paraproduct (Kovač 2012, Lemma 2). These provide a methodological precedent, rather than a bound for the present triangular form. In particular, Kovač explicitly identifies the obstruction to applying that framework to non-bipartite graphs, including the triangle, in (Kovač 2011, sec. 6.2). Here the energy is a trace of a matrix power, and the averaging is over the four children selected by the XOR constraint. The matrix energy and the dimension-independent trace inequality are taken from the companion manuscript (OpenAI 2026, secs. 2–3, Lemmas 2.1, 2.2 and 3.1); we reproduce their real finite-dimensional proofs. Their underlying matrix calculus is classical: the square-root derivative is a special case of the divided-difference formula in (Daletskii 1957, sec. 1, Equation (1)), and the order comparison uses monotonicity of the positive square root (Pedersen 1972, Theorem, p. 309). The energy argumentThe proof reduces the form to finite matrices by taking inputs constant on sufficiently small dyadic squares. On a fixed admissible triple, each input becomes a matrix between the atom spaces of its two variables. At each variable, we join its two incident matrices into a single row operator \(R\) and assign it the energy \(\mathop{\mathrm{tr}}((R^*R)^{3/2})\). Let \(e(\mathbf I)\) be the sum of these three energies, and let \(\operatorname{ch}(\mathbf I)\) consist of the four admissible triples obtained by halving each interval. The key estimate is \[ \lvert L_{\mathbf I}(F_0,F_1,F_2)\rvert \le C_0\,2^{2k} \left(\frac14\sum_{\mathbf I'\in\operatorname{ch}(\mathbf I)} e(\mathbf I')-e(\mathbf I)\right), \qquad \mathbf I\in\mathcal A_k, \tag{4}\] with an absolute constant \(C_0\). At each scale, the weighted total energy \(\sum_{\mathbf I\in\mathcal A_k}2^{2k}e(\mathbf I)\) is bounded by an absolute constant times the sum of the cubed input norms. To prove (4), a matrix trace estimate bounds the triangular product by three Hessian quadratic forms of \(P\mapsto\mathop{\mathrm{tr}}(P^{3/2})\). Conditional on one child half, each neighboring half remains equally likely to be left or right. The two neighbors are correlated, but \(RR^*\) is a sum of the two edge Gram matrices; it contains no product between their multipliers and has the same nonzero spectrum as \(R^*R\). Convexity therefore converts the Hessian bound into an increase of the child energy. Writing the local integrals in normalized interval measures leaves the weight \(2^{2k}\). Each child has one parent and weight \(2^{2(k-1)}\), one quarter of the parent’s weight, so these increases telescope. Section 2 establishes the energy inequalities, Section 3 proves the trace estimate, Section 4 supplies the conditional-averaging argument, and Section 5 sums the resulting differences and passes to measurable inputs. The matrix energy and its curvatureWe first record the finite-dimensional facts that will measure the energy increase under a dyadic split. All spaces and matrices in the proof are real; \(R^*\) denotes the transpose of \(R\). For a symmetric positive semidefinite matrix \(P\), define \[\Phi(P)=\mathop{\mathrm{tr}}(P^{3/2}),\qquad \mathop{\mathrm{supp}}P=(\ker P)^\perp.\] A symmetric matrix \(K\) is supported on \(P\) if it annihilates \(\ker P\). Symmetry then also puts its range in \(\mathop{\mathrm{supp}}P\). For such \(K\), define \[ b_P(K)=\frac32\sum_{i,j} \frac{\lvert K_{ij}\rvert^2}{\sqrt{p_i}+\sqrt{p_j}}, \tag{5}\] where \(p_i>0\) are the eigenvalues of \(P\) on its support, and the entries are taken in an orthonormal eigenbasis of that support. If \(P=0\), the only supported \(K\) is zero and \(b_0(0)=0\). Simultaneous orthogonal conjugation and extension by zero preserve \(\Phi\) and \(b\). The next two lemmas are the real-matrix versions of the energy derivative and order comparison results in the companion manuscript (OpenAI 2026, sec. 2). We give the proofs, including the support conventions needed for singular Gram matrices. Lemma 2 (Hessian of the energy). On matrices positive definite on a fixed support, \(\Phi\) is smooth and, for a symmetric direction \(K\) on that support, \[d\Phi_P(K)=\frac32\mathop{\mathrm{tr}}(\sqrt P\,K), \qquad d^2\Phi_P(K,K)=b_P(K).\] In particular, \(\Phi\) is convex on the positive semidefinite cone. Proof. Work on the support and set \(B=\sqrt P\). The derivative of the squaring map at \(B\) is \[\mathcal L_B(X)=BX+XB.\] This is the square-root instance of the classical matrix derivative calculus (Daletskii 1957, sec. 1, Equation (1)). In an eigenbasis of \(P\), this map multiplies entry \((i,j)\) by \(\sqrt{p_i}+\sqrt{p_j}>0\). The inverse function theorem therefore gives a smooth square root whose derivative \(X\) in direction \(K\) satisfies \(BX+XB=K\). Differentiating \(\mathop{\mathrm{tr}}(B^3)\) and using cyclicity, \[d\Phi_P(K)=3\mathop{\mathrm{tr}}(B^2X)=\frac32\mathop{\mathrm{tr}}(BK).\] A second differentiation gives \[d^2\Phi_P(K,K) =\frac32\langle K,\mathcal L_B^{-1}K\rangle_{\mathrm{HS}} =b_P(K),\] where \(\langle X,Y\rangle_{\mathrm{HS}}=\mathop{\mathrm{tr}}(X^*Y)\). The Hessian is nonnegative. This proves convexity on positive definite matrices; replacing each matrix by itself plus \(\eta\mathrm{Id}\) and letting \(\eta\downarrow0\) proves convexity on the closed cone. ◻ Lemma 3 (Order comparison). Suppose \(P,Q\) are positive semidefinite matrices on the same space, \(a\ge1\), and \(P\le aQ\). Every symmetric \(K\) supported on \(P\) is supported on \(Q\), and \[ b_P(K)\ge a^{-1/2}b_Q(K). \tag{6}\] Proof. For \(x\in\ker Q\), the inequalities \(0\le\langle Px,x\rangle\le a\langle Qx,x\rangle=0\) imply \(Px=0\). Thus \(\ker Q\subseteq\ker P\), which proves the support assertion. First suppose \(P,Q\) are positive definite. Inversion reverses positive definite order: conjugating \(0<X\le Y\) by \(X^{-1/2}\), inverting the resulting matrix at least \(\mathrm{Id}\), and conjugating back gives \(Y^{-1}\le X^{-1}\). The spectral integral \[\sqrt X=\frac1\pi\int_0^\infty X(X+t\mathrm{Id})^{-1}\,\frac{\mathrm dt}{\sqrt t}\] then proves monotonicity of the positive square root (Pedersen 1972, Theorem, p. 309), since \(X(X+t\mathrm{Id})^{-1}=\mathrm{Id}-t(X+t\mathrm{Id})^{-1}\). Consequently \(\sqrt P\le\sqrt a\,\sqrt Q\). For a positive semidefinite matrix \(A\), left and right multiplication by \(A\) are positive semidefinite self-adjoint operators on the full Hilbert–Schmidt matrix space: their quadratic forms are \(\mathop{\mathrm{tr}}(X^*AX)\) and \(\mathop{\mathrm{tr}}(X^*XA)\). Hence \[\mathcal L_{\sqrt P}\le\sqrt a\,\mathcal L_{\sqrt Q}, \qquad \mathcal L_{\sqrt P}^{-1} \ge a^{-1/2}\mathcal L_{\sqrt Q}^{-1}.\] Taking the quadratic form at \(K\) and using Lemma 2 proves (6). In the semidefinite case, \(a\ge1\) gives \(P+\eta\mathrm{Id}\le a(Q+\eta\mathrm{Id})\). Apply the positive definite result and let \(\eta\downarrow0\). In a full eigenbasis of either matrix, every entry of \(K\) meeting its kernel is zero. Formula (5) therefore gives convergence to the two supported quadratic forms in (6). ◻ Corollary 4 (A midpoint gap). If \(T\ge0\) and \(U=U^*\) satisfy \(-T\le U\le T\), then \(U\) is supported on \(T\) and \[ \frac{\Phi(T+U)+\Phi(T-U)}2-\Phi(T) \ge\frac{1}{2\sqrt2}b_T(U). \tag{7}\] Proof. For \(x\in\ker T\), positivity of \(T+U\) and \(T-U\), whose quadratic forms both vanish at \(x\), implies \(Ux=0\). For \(\lvert t\rvert<1\), \[(1-\lvert t\rvert)T\le T+tU\le(1+\lvert t\rvert)T\le2T.\] Thus \(T+tU\) has the same support as \(T\). The function \(f(t)=\Phi(T+tU)\) satisfies, by Lemmas 2 and 3, \[f''(t)=b_{T+tU}(U)\ge 2^{-1/2}b_T(U).\] Subtracting \(b_T(U)t^2/(2\sqrt2)\) leaves a convex function on \((-1,1)\), continuous on \([-1,1]\). Its midpoint inequality is (7). If \(T=0\), all terms are zero. ◻ A triangular trace estimateWe now compare a cyclic product of three matrices with the Hessian costs from Section 2. This is the finite-dimensional estimate that will control a local triangular integral. Its proof follows the mixed trace argument in (OpenAI 2026, sec. 3); working over the reals lets us identify the two orientations of the triangle directly by transposition. Let \(H_v\), \(v\in\mathbb Z/3\mathbb Z\), be finite-dimensional real inner product spaces, and let \(W_v:H_{v+1}\to H_v\). The two edges incident to vertex \(v\) form the row star \[ R_v=[\,W_v\quad W_{v-1}^*\,]: H_{v+1}\oplus H_{v-1}\longrightarrow H_v, \qquad T_v=R_v^*R_v. \tag{8}\] The two Gram matrices \(R_v^*R_v\) and \(R_vR_v^*\) have the same nonzero eigenvalues with multiplicities, so their \(\Phi\) values agree. Proposition 5 (Mixed trace estimate). For the maps in (8), let \(D_v:H_v\to H_v\) be symmetric with \(\lVert D_v\rVert_{\mathrm{op}}\le1\), and put \(U_v=R_v^*D_vR_v\). Then \(U_v\) is supported on \(T_v\), and \[ \lvert \mathop{\mathrm{tr}}(D_0W_0D_1W_1D_2W_2)\rvert \le\frac53\sum_{v=0}^2 b_{T_v}(U_v). \tag{9}\] The constant is independent of all three dimensions. Proof. The identity \(\ker T_v=\ker R_v\) proves the support assertion. We first place the three quadratic forms on one space, then bound a cubic trace in an eigenbasis. A common quadratic form.On \(H=H_0\oplus H_1\oplus H_2\), define \[M=\begin{pmatrix} 0&W_0&W_2^*\\ W_0^*&0&W_1\\ W_2&W_1^*&0 \end{pmatrix}, \qquad D=\mathop{\mathrm{diag}}(D_0,D_1,D_2).\] Both matrices are symmetric and \(\lVert D\rVert_{\mathrm{op}}\le1\). Let \(P_v\) be the projection onto \(H_v\), and set \(A_v=MP_vM\), \(K_v=MP_vDM\). The only nonzero block row of \(P_vM\) is \(R_v\), with its columns placed in vertex order. Thus \(A_v\) and \(K_v\) are \(T_v\) and \(U_v\), respectively, after a permutation of blocks and extension by zero. In particular \(K_v\) is supported on \(A_v\). Also \(P_vD=DP_v\), so \(K_v\) is symmetric, and \[0\le A_v\le M^2,\qquad \sum_vK_v=MDM.\] Lemma 3, followed by the quadratic-form inequality for a sum of three vectors, gives \[ \mathcal E:=\sum_v b_{T_v}(U_v) \ge\sum_v b_{M^2}(K_v) \ge\frac13b_{M^2}(MDM). \tag{10}\] This comparison is on the relevant supports; \(M\) need not be invertible. The cubic trace.Choose an orthonormal eigenbasis of \(M\), with eigenvalues \(m_i\) ordered so that \(q_i=\lvert m_i\rvert\) is nonincreasing. Write \(D_{ij}\) for the entries of \(D\) in this basis. Since \((MDM)_{ij}=m_im_jD_{ij}\), (10) gives \[ \mathcal E\ge\frac12 Q,\qquad Q=\sum_{\substack{i,j\\q_i+q_j>0}} \frac{q_i^2q_j^2}{q_i+q_j}\lvert D_{ij}\rvert^2. \tag{11}\] Define \[A_i=q_i^3\lvert D_{ii}\rvert^2,\qquad E_i=q_i\sum_{j>i}q_j^2\lvert D_{ij}\rvert^2,\qquad A=\sum_iA_i,\quad E=\sum_iE_i.\] The diagonal terms of \(Q\) sum to \(A/2\). Pairing its off-diagonal terms and using \(q_i\ge q_j\) for \(i<j\), we obtain \[ Q=\frac A2+ \sum_{\substack{i<j\\q_i+q_j>0}} \frac{2q_i^2q_j^2}{q_i+q_j}\lvert D_{ij}\rvert^2 \ge \frac A2+E. \tag{12}\] Expand \[\mathop{\mathrm{tr}}((DM)^3)=\sum_{i,j,k}m_im_jm_kD_{ij}D_{jk}D_{ki}.\] Group the triples by their smallest index \(i\) and the number of times it occurs. If it occurs once, its three possible positions give \[3m_i\sum_{j,k>i}m_jm_kD_{ij}D_{jk}D_{ki} =3m_i x^*D_{>i}x,\qquad x_j=m_jD_{ji}.\] Here \(j=k\) is allowed, and \(D_{>i}\) is the compression of \(D\) to indices greater than \(i\). This compression is a contraction, so the absolute value is at most \(3E_i\). If the smallest index occurs twice, the contribution is \[3m_i^2D_{ii}\sum_{j>i}m_j\lvert D_{ij}\rvert^2.\] The row norm bound \(\sum_j\lvert D_{ij}\rvert^2\le1\) and Cauchy–Schwarz show that its absolute value is at most \[3q_i^2\lvert D_{ii}\rvert \left(\sum_{j>i}q_j^2\lvert D_{ij}\rvert^2\right)^{1/2} =3\sqrt{A_iE_i}.\] When all three indices equal \(i\), the absolute value is at most \(A_i\), since \(\lvert D_{ii}\rvert\le1\). These cases partition all triples, including repeated indices. Summing and applying Cauchy–Schwarz once more, \[ \begin{split} \lvert \mathop{\mathrm{tr}}((DM)^3)\rvert &\le A+3E+3\sqrt{AE}\\ &\le \tfrac52A+\tfrac92E \le 5(A/2+E)\le5Q. \end{split} \tag{13}\] Zero eigenvalues contribute zero throughout. Returning to the triangle.In vertex blocks, a nonzero closed three-step product must visit all three vertices because \(M\) has zero diagonal blocks. The three starting points in one orientation give \(\tau=\mathop{\mathrm{tr}}(D_0W_0D_1W_1D_2W_2)\) by cyclicity, and the reverse orientation gives the same real trace by transposition. Thus \(\mathop{\mathrm{tr}}((DM)^3)=6\tau\). Equations (11) and (13) yield \[6\lvert \tau\rvert\le5Q\le10\mathcal E,\] which is (9). ◻ Energy increase under a dyadic splitWe apply the matrix estimate to a fixed admissible triple and compare its energy with the average energy of its children. For this section, the inputs are bounded, compactly supported, and constant on products of intervals in \(\mathcal D_m\), for some \(m\in\mathbb Z\). Matrices for a local integralFor \(\mathbf I=(I_0,I_1,I_2)\in\mathcal A_k\), \(k\ge m\), let \(H_v\) have an orthonormal basis indexed by the intervals of \(\mathcal D_m\) inside \(I_v\). Call these intervals atoms. In the probability measure \(\lvert I_v\rvert^{-1}\,\mathrm dx_v\), each atom has weight \(w_v(i)=2^{m-k}\). Define \(W_v:H_{v+1}\to H_v\) by \[ W_v(i,j)=\sqrt{w_v(i)w_{v+1}(j)}\,F_v(i,j), \tag{14}\] where \(F_v(i,j)\) is the constant value on the corresponding atom pair. Use these maps in (8), and define \[ e_v(\mathbf I)=\Phi(T_v)=\Phi(R_vR_v^*), \qquad e(\mathbf I)=\sum_{v=0}^2 e_v(\mathbf I). \tag{15}\] If \(k\ge m+1\), let \(D_v\) be the diagonal matrix of the \(h_{I_v}\)-values on the atoms, and put \[\tau(\mathbf I)=\mathop{\mathrm{tr}}(D_0W_0D_1W_1D_2W_2).\] The diagonal matrices are symmetric contractions. In the expanded trace, each vertex weight occurs as two square roots, so \(\tau(\mathbf I)\) is exactly the normalized integral of the product of the three inputs and three Haar signs. Therefore \[ L_{\mathbf I}(F_0,F_1,F_2)=2^{2k}\tau(\mathbf I). \tag{16}\] The four childrenIf \(b_v\in\{0,1\}\) chooses the left or right half of \(I_v\), the child index is \(2n_{I_v}+b_v\). The child triple is admissible precisely when \(b_0\oplus b_1\oplus b_2=0\). Equivalently, with \(s_v=(-1)^{b_v}\), its signs satisfy \(s_0s_1s_2=1\). Write \(\operatorname{ch}(\mathbf I)\) for these four children. Under uniform choice among them, each sign is uniform and every pair of signs is independent. Figure 1 displays the conditional averages used below. Proposition 6 (Local energy increase). For \(\mathbf I\in\mathcal A_k\), \(k\ge m+1\), define \[\delta(\mathbf I) =\frac14\sum_{\mathbf I'\in\operatorname{ch}(\mathbf I)} e(\mathbf I')-e(\mathbf I).\] Then \(\delta(\mathbf I)\ge0\), and \[ \lvert \tau(\mathbf I)\rvert \le\frac{10\sqrt2}{3}\,\delta(\mathbf I). \tag{17}\] Proof. We keep the parent spaces fixed and extend each child matrix by zero. Set \[C_v=(\mathrm{Id}+s_vD_v)^{1/2}.\] It is \(\sqrt2\) times the projection onto the atoms in the chosen half. Child probability weights double, so the extended child edge matrix is \(C_vW_vC_{v+1}\). Its row star is \[R_v(s)=C_vR_v\mathop{\mathrm{diag}}(C_{v+1},C_{v-1}).\] In particular, \[ R_v(s)R_v(s)^* =C_v\bigl( W_vC_{v+1}^2W_v^* +W_{v-1}^*C_{v-1}^2W_{v-1} \bigr)C_v. \tag{18}\] Fix \(s_v\). Each neighboring sign is still uniform, so its squared multiplier has conditional expectation \(\mathrm{Id}\). Although the neighbors are correlated, (18) has no product between their multipliers. Thus \[\mathbb E\bigl[R_v(s)R_v(s)^*\mid s_v\bigr] =C_vR_vR_v^*C_v.\] By the convexity in Lemma 2, \[ \mathbb E\bigl[e_v(\mathbf I(s))\mid s_v\bigr] \ge\Phi(C_vR_vR_v^*C_v) =\Phi(T_v+s_vU_v), \qquad U_v=R_v^*D_vR_v. \tag{19}\] The equality compares the two Gram matrices of \(C_vR_v\): their nonzero eigenvalues agree, even though they act on different spaces. Since \(D_v\) is a symmetric contraction, \(-T_v\le U_v\le T_v\). Averaging (19) over \(s_v=\pm1\) and applying Corollary 4 gives \[\frac14\sum_{\mathbf I'\in\operatorname{ch}(\mathbf I)} e_v(\mathbf I')-e_v(\mathbf I) \ge\frac{1}{2\sqrt2}b_{T_v}(U_v).\] Summing over \(v\) proves nonnegativity of \(\delta\). Proposition 5 now gives \[\lvert \tau(\mathbf I)\rvert \le\frac53\sum_v b_{T_v}(U_v) \le\frac{10\sqrt2}{3}\delta(\mathbf I),\] as asserted. ◻ Summation and passage to measurable inputsThe local increase from Proposition 6 has the sign needed for telescoping toward finer scales. This use of an energy difference parallels the Bellman-function summations in (Kovač 2011, sec. 2) and (Kovač 2012, Lemma 2). We bound the total energy at each level before carrying out that sum. Lemma 7 (Total energy). For the step functions of Section 4 and every \(k\ge m\), set \[J_k=\sum_{\mathbf I\in\mathcal A_k}2^{2k}e(\mathbf I).\] Then \[ 0\le J_k\le2\sqrt2\sum_{v=0}^2\lVert F_v\rVert_3^3. \tag{20}\] For \(k\ge m+1\), \[ \sum_{\mathbf I\in\mathcal A_k}2^{2k}\delta(\mathbf I) =J_{k-1}-J_k. \tag{21}\] Proof. If \(a,b\) are the Hilbert–Schmidt norms of the two edges incident to \(v\), then \[e_v(\mathbf I) =\mathop{\mathrm{tr}}(T_v^{3/2}) \le(\mathop{\mathrm{tr}}T_v)^{3/2} =(a^2+b^2)^{3/2} \le\sqrt2(a^3+b^3).\] For an edge \(W_v\), its probability normalization gives \[ \lVert W_v\rVert_{\mathrm{HS}}^3 =\left(\frac1{\lvert I_v\rvert\lvert I_{v+1}\rvert} \int_{I_v\times I_{v+1}}\lvert F_v\rvert^2\right)^{3/2} \le \frac1{\lvert I_v\rvert\lvert I_{v+1}\rvert} \int_{I_v\times I_{v+1}}\lvert F_v\rvert^3. \tag{22}\] Every edge occurs in two row stars. Also, every ordered pair of intervals in \(\mathcal D_k\) determines exactly one admissible third interval, by XOR. Multiplication by \(2^{2k}=\lvert I_v\rvert\lvert I_{v+1}\rvert\) and summation of (22) therefore prove (20). These sums are finite: compact support leaves finitely many nonzero edge matrices, each belonging to one admissible triple. Deleting the last bit of each child index shows that every admissible child has a unique admissible parent. As \(2^{2k}/4=2^{2(k-1)}\), the child part in the definition of \(\delta\) sums to \(J_{k-1}\), proving (21). ◻ Proof of Theorem 1 for step functions. The case \(S=\varnothing\) is immediate. Otherwise set \(k_-=\min S\), \(k_+=\max S\), and refine the common atom level, if necessary, so that \(m\le k_--1\). By (16), Proposition 6, and Lemma 7, \[\begin{align*} \sum_{k\in S}\sum_{\mathbf I\in\mathcal A_k}\lvert L_{\mathbf I}(F_0,F_1,F_2)\rvert &\le\frac{10\sqrt2}{3} \sum_{k=k_-}^{k_+}(J_{k-1}-J_k)\\ &\le\frac{10\sqrt2}{3}J_{k_--1} \le\frac{40}{3}\sum_{v=0}^2\lVert F_v\rVert_3^3. \end{align*}\] The insertion of missing scales is valid because each energy difference is nonnegative. If every input has nonzero norm, apply this estimate to \(F_v/\lVert F_v\rVert_3\). Trilinearity of each local integral gives (3), with constant \(40\). If any norm is zero, the local integrals vanish. ◻ To pass to general inputs we need continuity of the absolute sum, not merely continuity of the signed form. The following fixed-level estimate provides it. Lemma 8 (Continuity at one scale). For every \(k\in\mathbb Z\) and real \(F_v\in L^3(\mathbb R_+^2)\), \[ \sum_{\mathbf I\in\mathcal A_k}\lvert L_{\mathbf I}(F_0,F_1,F_2)\rvert \le\prod_{v=0}^2\lVert F_v\rVert_3. \tag{23}\] Consequently the sequence \((L_{\mathbf I}(F_0,F_1,F_2))_{\mathbf I\in\mathcal A_k}\) depends continuously on the inputs as a map from \(L^3\times L^3\times L^3\) to \(\ell^1(\mathcal A_k)\). Proof. Define the nonnegative edge averages \[a_v(\mathbf I)= \frac1{\lvert I_v\rvert\lvert I_{v+1}\rvert} \int_{I_v\times I_{v+1}}\lvert F_v\rvert^3.\] Hölder’s inequality on the product probability space of the three intervals, with the Haar signs bounded by one, gives \[\lvert L_{\mathbf I}(F_0,F_1,F_2)\rvert \le2^{2k}\prod_{v=0}^2 a_v(\mathbf I)^{1/3}.\] Apply Hölder again, now to the sum over \(\mathcal A_k\) with weight \(2^{2k}\). The uniqueness of the third interval yields \[\sum_{\mathbf I\in\mathcal A_k}2^{2k}a_v(\mathbf I)=\lVert F_v\rVert_3^3,\] proving (23). These bounds also justify all integrals and absolute sums for \(L^3\) inputs. For two input triples \(F,G\), expand the difference of local integrals into the three terms with inputs \[(F_0-G_0,F_1,F_2),\quad (G_0,F_1-G_1,F_2),\quad (G_0,G_1,F_2-G_2).\] Estimate each term by (23). If \(G_v\to F_v\) in \(L^3\), the sum of these three product bounds tends to zero. This is the asserted \(\ell^1\) continuity. ◻ Completion of Theorem 1. Bounded compactly supported dyadic step functions are dense in \(L^3(\mathbb R_+^2)\). To see this, first approximate an \(L^3\) function by a continuous compactly supported function, then take its averages on sufficiently small dyadic squares. Uniform continuity and a common bounded support give convergence in \(L^3\). For arbitrary real \(F_v\in L^3\), choose such step functions \(F_v^{(n)}\to F_v\) in \(L^3\). Assuming \(S\ne\varnothing\), refine their common atom levels, without changing the functions, to satisfy \(m_n\le\min S-1\). Apply the step-function estimate to these inputs. Lemma 8, summed over the fixed finite set \(S\), gives convergence of their local integrals in \(\ell^1\). The inequality \(\lvert \lvert a\rvert-\lvert b\rvert\rvert\le\lvert a-b\rvert\) permits passage to the absolute sum in (3), and norm convergence handles its right-hand side. This proves the theorem and its stated extension to real \(L^3\) inputs. The case \(S=\varnothing\) remains immediate. For any coefficients \(\lvert \epsilon_{\mathbf I}\rvert\le1\), the triangle inequality gives the corresponding bound for \[\sum_{k\in S}\sum_{\mathbf I\in\mathcal A_k} \epsilon_{\mathbf I}L_{\mathbf I}(F_0,F_1,F_2). \qedhere\] ◻
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