\chapter{Saturated tree vectors and the product inequality}\label{sec:geometry-results} This section and the next concern the cubic model. In this section, we study unit vectors of the tree Hilbert space whose cubic tree energy is close to the ceiling $\Eth$ of \cref{thm:geometry-tree-ceiling}. We prove two results about such vectors. The first, \cref{thm:geometry-universal-root}, states that the root operator $\mathcal I^*v$ of a vector close to the ceiling is close, in suitable coordinates, to one universal integral operator on $L^2(0,1)$. The second, \cref{thm:geometry-threshold-product}, is a product inequality for three such vectors whose overlaps are nonnegative at every height. \Cref{lem:geometry-coherent-root,lem:geometry-pair-deficit} are the intermediate steps. The section is deterministic. It uses the tree Hilbert space of \cref{sec:geometry-core} and the cubic ceiling of \cref{thm:geometry-tree-ceiling}, with the retained defects \eqref{eq:geometry-height-defect} and \eqref{eq:geometry-angular-young-defects} proved in \cref{sec:tree-ceilings}. Nothing about the CK equations is used. In \cref{sec:three-time}, we apply both theorems to the normalized prefix centers of the cubic CK solution: \cref{thm:geometry-threshold-product} gives the three-time product inequality of \cref{thm:geometry-actual-product}, and \cref{thm:geometry-universal-root} is the main input of the susceptibility bound in \cref{thm:geometry-susceptibility-lower}. \paragraph{Notation.} Throughout this section, $p=3$, so that the grafting map $\mathcal I\colon\mathcal H\otimes\mathcal H\to\mathcal H$ is binary. Recall from \cref{sec:geometry-core} that $\mathcal H$ is a real separable Hilbert space, that $\mathcal I$ is an isometry, and that its range is the orthogonal complement of the one-leaf summand. The one-leaf summand is the subspace of height zero, and we have \begin{equation}\label{eq:geometry-graft-range} \mathcal I\mathcal I^*=\Id-\Pi_0 . \end{equation} We write $\Pi_j$ for the projection onto trees of height exactly $j$ and $\Pi_{\le H}=\sum_{j=0}^H\Pi_j$; the projections $\Pi_j$ are orthogonal and sum to the identity. As in \cref{sec:geometry-core}, we identify a tensor $x\otimes y$ with the Hilbert--Schmidt operator $|x\rangle\langle y|$, which maps $z$ to $\ip{y}{z} x$. Then $\mathcal I^*v$ is a Hilbert--Schmidt operator on $\mathcal H$, and $\norm{\mathcal I^*v}_{\HS}\le\norm{v}$. We write $\ip{A}{B}_{\HS}=\tr(A^*B)$, so that \[ \bigl\langle |a\rangle\langle b|,|c\rangle\langle d|\bigr\rangle_{\HS} =\ip{a}{c}\ip{b}{d} . \] For $v\in\mathcal H$, let \[ f(v)=\ip{v}{\mathcal I(v\otimes v)} =\bigl\langle\mathcal I^*v,|v\rangle\langle v|\bigr\rangle_{\HS}, \qquad F_*=\frac{2\sqrt2}{3}, \] and, for a unit vector $v$, let $\delta(v)=F_*-f(v)$ be its \emph{deficit}. By \cref{thm:geometry-tree-ceiling}, we have $\delta(v)>0$ for every unit vector $v$. The cubic tree energy of \eqref{eq:geometry-tree-energy} is $h(v)=\sqrt3 f(v)$, and $\Eth=\sqrt3F_*$. Hence the deficit $\delta(v)=(\Eth-h(v))/\sqrt3$ is the energy deficit divided by $\sqrt3$. For a unit vector $v$, we use the height masses of \cref{thm:geometry-tree-ceiling}: \[ v_j=\Pi_jv,\qquad b_j=\norm{v_j}^2,\qquad B_j=\sum_{i\le j}b_i,\qquad a_j=\sqrt{b_j},\qquad \bar b=\sup_{j\ge0}b_j, \] with $B_{-1}=B_{-2}=0$. Note that $B_j\uparrow1$ as $j\to\infty$. \paragraph{The height rule.} A graft has height one plus the larger of the heights of its two children. This means that $\mathcal I$ maps $\Pi_i\mathcal H\otimes\Pi_k\mathcal H$ into $\Pi_{\max(i,k)+1}\mathcal H$, and \begin{equation}\label{eq:geometry-height-rule} \Pi_j\mathcal I(x\otimes y)=\sum_{\max(i,k)=j-1}\mathcal I(\Pi_ix\otimes\Pi_ky)\quad(j\ge1), \qquad \Pi_0\mathcal I=0 . \end{equation} Taking adjoints, we find that $\mathcal I^*\Pi_0=0$ and, for $j\ge1$, \begin{equation}\label{eq:geometry-root-blocks} \mathcal I^*\Pi_jv=\sum_{\max(i,k)=j-1}\Pi_i(\mathcal I^*v)\Pi_k . \end{equation} In words, the height-$j$ component of $v$ is carried by the blocks $\Pi_i(\mathcal I^*v)\Pi_k$ of the root operator with $\max(i,k)=j-1$. We call $j$ the \emph{root height} of these blocks. Blocks with different root heights are orthogonal in the Hilbert--Schmidt inner product, and the restriction of $\mathcal I^*$ to $\Pi_j\mathcal H$ is an isometry for $j\ge1$, by \eqref{eq:geometry-graft-range}. \paragraph{The retained defects.} Let $v$ be a unit vector with deficit $\delta$. By \eqref{eq:geometry-height-rule} and the isometry of $\mathcal I$ (see also \cref{lem:tree-graft-heights}), the projected graft $g_j=\Pi_j\mathcal I(v\otimes v)$ satisfies \begin{equation}\label{eq:geometry-graft-norm} \norm{g_j}^2=\sum_{\max(i,k)=j-1}b_ib_k=B_{j-1}^2-B_{j-2}^2=b_{j-1}s_j^2, \qquad s_j=\sqrt{B_{j-1}+B_{j-2}} . \end{equation} Let $\theta_j$ be the angle between $v_j$ and $g_j$, with the convention $\cos\theta_j=1$ when $v_j=0$ or $g_j=0$. We use three consequences of \cref{thm:geometry-tree-ceiling}. The first inequality in \eqref{eq:geometry-height-defect} implies that \begin{equation}\label{eq:geometry-mesh-bound} \bar b\le\Bigl(\sum_{j\ge0}b_j^2\Bigr)^{1/2}\le(4\sqrt2\,\delta)^{1/2}=2^{5/4}\delta^{1/2}, \end{equation} and \eqref{eq:geometry-angular-young-defects} states that \begin{equation}\label{eq:geometry-retained-recalled} \sum_{j\ge1}a_ja_{j-1}s_j(1-\cos\theta_j)\le\delta, \qquad \frac12\sum_{j\ge1}s_j(a_j-a_{j-1})^2\le\delta . \end{equation} \section{The universal operator at a saturated root} By \eqref{eq:geometry-mesh-bound}, a vector close to the ceiling has small mass at every height. The retained defects \eqref{eq:geometry-retained-recalled} give more information: they bound weighted sums of the variations $a_j-a_{j-1}$ of the height amplitudes and of the angular errors $1-\cos\theta_j$ between $v_j$ and the projected graft $g_j$ of the lower components. The next lemma shows that, as a consequence, the root operator of $v$ is close to an operator whose coefficients in the normalized height directions $v_j/\sqrt{b_j}$, for $b_j>0$, depend only on the height masses. \begin{lemma}[Coherent approximation of a root] \label{lem:geometry-coherent-root} Let $v$ be a unit tree vector with $\delta=\delta(v)\le1$. There exists a symmetric Hilbert--Schmidt operator $\widetilde A_v$ with $\norm{\widetilde A_v}_{\HS}=1$ and height blocks \begin{equation} \Pi_i\widetilde A_v\Pi_k =\frac{|v_i\rangle\langle v_k|}{\sqrt{B_h+B_{h-1}}},\qquad h=\max(i,k), \label{eq:geometry-coherent-root-blocks} \end{equation} where a zero denominator means a zero block, such that \begin{equation} \norm{\mathcal I^*v-\widetilde A_v}_{\HS}\le K\delta^{1/4}. \label{eq:geometry-coherent-root-error} \end{equation} Here $K$ is an absolute constant; one can take $K=5$. \end{lemma} \begin{proof} The proof has three steps. First, we define $\widetilde A_v$ one root height at a time and compute its norm. Second, we compute the error at each root height. Third, we sum the errors: at root heights above a small cumulative mass $\varepsilon$, we use the retained defects; the remaining root heights form an initial segment of small mass. \paragraph{Step 1: definition and normalization.} For $j\ge1$, let $g_j$ and $s_j$ be as in \eqref{eq:geometry-graft-norm}. We define the component of $\widetilde A_v$ at root height $j$ by \[ \widetilde A^{(j)}=\frac{\mathcal I^*g_j}{s_j}\quad\text{if } s_j>0, \qquad \widetilde A^{(j)}=0\quad\text{if } s_j=0, \] and we set $\widetilde A_v=\sum_{j\ge1}\widetilde A^{(j)}$. Using \eqref{eq:geometry-height-rule} and $\mathcal I^*\mathcal I=\Id$, we have \[ \mathcal I^*g_j=\sum_{\max(i,k)=j-1}|v_i\rangle\langle v_k| . \] With $h=j-1$, the denominator $s_j$ equals $\sqrt{B_h+B_{h-1}}$, and the blocks of $\widetilde A_v$ are those in \eqref{eq:geometry-coherent-root-blocks}. The block with indices $(k,i)$ is the adjoint of the block with indices $(i,k)$, and therefore $\widetilde A_v$ is symmetric. By \eqref{eq:geometry-graft-norm} and the isometry of $\mathcal I$, we have $\norm{\widetilde A^{(j)}}_{\HS}^2=\norm{g_j}^2/s_j^2=b_{j-1}$ when $s_j>0$. When $s_j=0$, we have $B_{j-1}=0$, and in particular $b_{j-1}=0$. The components with different root heights are orthogonal. Summing over $j$, we find \[ \norm{\widetilde A_v}_{\HS}^2=\sum_{j\ge1}b_{j-1}=\sum_{h\ge0}b_h=1 . \] \paragraph{Step 2: the error at one root height.} By \eqref{eq:geometry-root-blocks}, we have $\mathcal I^*v=\sum_{j\ge1}\mathcal I^*v_j$, and $\mathcal I^*v_j$ lies in the same root-height component as $\widetilde A^{(j)}$. By orthogonality, \[ \norm{\mathcal I^*v-\widetilde A_v}_{\HS}^2=\sum_{j\ge1}\norm{\mathcal I^*v_j-\widetilde A^{(j)}}_{\HS}^2 . \] For $j\ge1$, the vector $v_j$ lies in the range of $\mathcal I$, and \eqref{eq:geometry-graft-range} gives $\norm{\mathcal I^*v_j}_{\HS}^2=b_j$. If $s_j>0$, then, since $g_j$ also lies in the range of $\mathcal I$, \[ \bigl\langle\mathcal I^*v_j,\widetilde A^{(j)}\bigr\rangle_{\HS} =\frac{\ip{v_j}{\mathcal I\mathcal I^*g_j}}{s_j} =\frac{\ip{v_j}{g_j}}{s_j} =a_ja_{j-1}\cos\theta_j, \] where we used $\norm{g_j}=a_{j-1}s_j$ from \eqref{eq:geometry-graft-norm}. The error at root height $j$ is \begin{equation}\label{eq:geometry-root-height-error} \norm{\mathcal I^*v_j-\widetilde A^{(j)}}_{\HS}^2 =b_j+b_{j-1}-2a_ja_{j-1}\cos\theta_j =(a_j-a_{j-1})^2+2a_ja_{j-1}(1-\cos\theta_j). \end{equation} If $s_j=0$, then $b_{j-1}=0$ and the error is $b_j$, in agreement with \eqref{eq:geometry-root-height-error}. \paragraph{Step 3: summation.} If $\delta=1$, then \eqref{eq:geometry-coherent-root-error} holds with $K=2$, because both operators have Hilbert--Schmidt norm at most one. We assume from now on that $\delta<1$. Fix $\varepsilon\in(0,1)$. We first consider the root heights $j\ge1$ with $B_{j-2}\ge\varepsilon$. For these, $s_j^2=B_{j-1}+B_{j-2}\ge2\varepsilon$. Multiplying each term of \eqref{eq:geometry-root-height-error} by $s_j/\sqrt{2\varepsilon}\ge1$ and using \eqref{eq:geometry-retained-recalled}, we obtain \[ \sum_{j:\,B_{j-2}\ge\varepsilon}\norm{\mathcal I^*v_j-\widetilde A^{(j)}}_{\HS}^2 \le\frac1{\sqrt{2\varepsilon}}\sum_{j\ge1}s_j\Bigl[(a_j-a_{j-1})^2+2a_ja_{j-1}(1-\cos\theta_j)\Bigr] \le\frac{4\delta}{\sqrt{2\varepsilon}} . \] The remaining root heights form an initial segment. Let $m_\varepsilon=\min\{k\ge0:B_k\ge\varepsilon\}$, which is finite because $B_k\uparrow1$. The condition $B_{j-2}<\varepsilon$ holds exactly when $1\le j\le m_\varepsilon+1$, because $B$ is nondecreasing. On this segment, \[ \sum_{j=1}^{m_\varepsilon+1}b_j\le B_{m_\varepsilon-1}+b_{m_\varepsilon}+b_{m_\varepsilon+1}\le\varepsilon+2\bar b, \qquad \sum_{j=1}^{m_\varepsilon+1}b_{j-1}=B_{m_\varepsilon}\le\varepsilon+\bar b . \] Using $\norm{x-y}^2\le2\norm{x}^2+2\norm{y}^2$ together with $\norm{\mathcal I^*v_j}_{\HS}^2=b_j$ and $\norm{\widetilde A^{(j)}}_{\HS}^2=b_{j-1}$, we find that the errors on this segment sum to at most $4\varepsilon+6\bar b$. Adding the two bounds and using \eqref{eq:geometry-mesh-bound}, we obtain \[ \norm{\mathcal I^*v-\widetilde A_v}_{\HS}^2 \le4\varepsilon+6\cdot2^{5/4}\delta^{1/2}+\frac{4\delta}{\sqrt{2\varepsilon}} . \] We choose $\varepsilon=\delta^{1/2}$. Then $\delta^{3/4}\le\delta^{1/2}$, because $\delta<1$, and the right side is at most $(4+6\cdot2^{5/4}+2\sqrt2)\delta^{1/2}\le25\delta^{1/2}$. This proves \eqref{eq:geometry-coherent-root-error} with $K=5$. \end{proof} When the height mesh $\bar b$ is small, the denominator in \eqref{eq:geometry-coherent-root-blocks} is close to $\sqrt{2B_h}$, and $B_h$ varies almost continuously with the height. In the coordinate $x=B_h$ on $(0,1)$, the blocks then become the values of one function of two variables. This is the content of the next theorem. \begin{theorem}[Universal threshold root] \label{thm:geometry-universal-root} Let $\mathcal K$ be a fixed separable infinite-dimensional Hilbert space, and let $\mathbf1$ denote the constant function one in $L^2(0,1)$. If $\norm{v_n}=1$ and $f(v_n)\to F_*$, then there exist isometric embeddings $V_n\colon\mathcal H\to L^2(0,1)\oplus\mathcal K$ satisfying $V_nv_n=\mathbf1$, for which \begin{equation} V_n\mathcal I^*v_nV_n^*\longrightarrow\mathcal T\oplus0 \quad\text{in Hilbert--Schmidt norm}, \qquad T(x,y)=\frac1{\sqrt{2\max(x,y)}} . \label{eq:geometry-universal-root} \end{equation} Here $\mathcal T$ is the integral operator on $L^2(0,1)$ with kernel $T$. The operator $\mathcal T$ is positive and trace class, with the positive frame \begin{equation} \mathcal T=\frac1{\sqrt2}|\mathbf1\rangle\langle\mathbf1| +\frac1{2\sqrt2}\int_0^1z^{-3/2} |\mathbf1_{[0,z]}\rangle\langle\mathbf1_{[0,z]}|\,\dd z . \label{eq:geometry-universal-root-frame} \end{equation} In particular, $\tr\mathcal T=\sqrt2$ and $\norm{\mathcal T}_{\HS}=1$. \end{theorem} \begin{remark}[Interpretation of the universal kernel]\label{rem:geometry-universal-kernel} In the coordinates of \cref{thm:geometry-universal-root}, a point $x\in(0,1)$ stands for the height at which the cumulative squared mass of $v_n$ reaches $x$. The kernel says that, at the threshold, the root of $v_n$ couples two children at cumulative masses $x$ and $y$ with a weight that depends only on the larger of the two, that is, on the taller child. In this continuum description, the weight $(2\max(x,y))^{-1/2}$ is, up to null sets, the unique nonnegative function of $\max(x,y)$ that gives squared root mass $\dd x$ to each band of cumulative mass $\dd x$: the pairs $(x',y')$ with $\max(x',y')\in[x,x+\dd x]$ have area $2x\,\dd x$, and $T^2\cdot2x\,\dd x=\dd x$. (At a finite root height $j$, the coherent approximation of \cref{lem:geometry-coherent-root} carries the squared mass $b_{j-1}$ of the height below.) The threshold value itself is the quadratic form of $\mathcal T$ on the constant function: \[ \ip{\mathbf1}{\mathcal T\mathbf1}=2\int_0^1\frac{x}{\sqrt{2x}}\,\dd x=\frac{2\sqrt2}3=F_* . \] This is consistent with $f(v_n)=\langle\mathcal I^*v_n,|v_n\rangle\langle v_n|\rangle_{\HS}\to F_*$. The convergence \eqref{eq:geometry-universal-root} holds in Hilbert--Schmidt norm only, and we do not claim that the traces of the operators $\mathcal I^*v_n$ converge to $\tr\mathcal T$. For this reason, \cref{sec:geometry-susceptibility} uses the frame \eqref{eq:geometry-universal-root-frame} only through the lower semicontinuity of the trace. \end{remark} \begin{proof}[Proof of \cref{thm:geometry-universal-root}] The proof has six steps. After a bound on the height mesh, we embed each $v_n$ so that its heights become consecutive intervals of $(0,1)$. In these coordinates, the coherent approximation of \cref{lem:geometry-coherent-root} becomes an integral operator with a step kernel. We then replace the step kernel by a simpler one and show that it converges to $T$. In the last step, we prove the properties of $\mathcal T$. We write $\delta_n=\delta(v_n)$, and $b_{n,j}$, $B_{n,j}$, and $\bar b_n$ for the height masses of $v_n$. When no confusion can arise, we drop the index $n$. \paragraph{Step 1: the height mesh.} By \eqref{eq:geometry-mesh-bound}, we have $\bar b_n\le2^{5/4}\delta_n^{1/2}$, which tends to zero because $\delta_n\to0$. \paragraph{Step 2: the embedding.} For each $j$ with $b_j>0$, let $\hat v_j=v_j/\sqrt{b_j}$ and $J_j=(B_{j-1},B_j)$. The vectors $\hat v_j$ are orthonormal, and so are the functions $b_j^{-1/2}\mathbf1_{J_j}$, because the intervals $J_j$ are disjoint and have lengths $b_j$. Let $E_n$ be the closed span of the vectors $\hat v_j$, and let $W_n\colon E_n\to L^2(0,1)$ be the isometry with $W_n\hat v_j=b_j^{-1/2}\mathbf1_{J_j}$. The orthogonal complement $E_n^\perp$ is separable, because $\mathcal H$ is separable (it is a countable direct sum of tensor powers of a separable space). It is also infinite-dimensional, because it contains every vector of the one-leaf summand that is orthogonal to $\hat v_0$ (or the whole summand if $b_0=0$), and the one-leaf summand is infinite-dimensional by \cref{sec:tree-space}. We may therefore choose a unitary map $U_n\colon E_n^\perp\to\mathcal K$. We define $V_n(x+y)=W_nx\oplus U_ny$ for $x\in E_n$ and $y\in E_n^\perp$. Then $V_n$ is an isometry, and \[ V_nv_n=\sum_{j:\,b_j>0}\sqrt{b_j}\,W_n\hat v_j=\sum_{j:\,b_j>0}\mathbf1_{J_j}=\mathbf1, \] since the intervals $J_j$ cover $(0,1)$ up to a countable set. Conjugation by $V_n$ preserves Hilbert--Schmidt norms, positivity, and traces, because $V_n^*V_n$ is the identity of $\mathcal H$. Further, $V_n|x\rangle\langle y|V_n^*=|V_nx\rangle\langle V_ny|$. \paragraph{Step 3: the coherent approximation as a step kernel.} Let $\widetilde A_n=\widetilde A_{v_n}$ be the operator of \cref{lem:geometry-coherent-root}, which applies once $\delta_n\le1$. Since $V_nv_{n,i}=\mathbf1_{J_i}$, the blocks \eqref{eq:geometry-coherent-root-blocks} are transported to \[ V_n\frac{|v_{n,i}\rangle\langle v_{n,k}|}{\sqrt{B_h+B_{h-1}}}V_n^* =\frac{|\mathbf1_{J_i}\rangle\langle\mathbf1_{J_k}|}{\sqrt{B_h+B_{h-1}}}, \qquad h=\max(i,k). \] In other words, $V_n\widetilde A_nV_n^*$ is the integral operator on $L^2(0,1)$, extended by zero on $\mathcal K$, with the step kernel \[ \widetilde T_n(x,y)=\frac1{\sqrt{B_h+B_{h-1}}},\qquad x\in J_i,\ y\in J_k,\ h=\max(i,k). \] Recall that the Hilbert--Schmidt norm of an integral operator is the $L^2$ norm of its kernel. Then \cref{lem:geometry-coherent-root} implies that \[ \norm{V_n\mathcal I^*v_nV_n^*-\widetilde T_n}_{\HS}=\norm{\mathcal I^*v_n-\widetilde A_n}_{\HS}\le5\delta_n^{1/4}\to0 . \] Here and below, we identify a kernel with its integral operator. \paragraph{Step 4: replacement of the denominator.} Let $T_n$ be the step kernel equal to $(2B_h)^{-1/2}$ on $J_i\times J_k$, with $h=\max(i,k)$. The set of pairs $(x,y)$ with $\max(i,k)=h$ has area $\sum_{\max(i,k)=h}b_ib_k=B_h^2-B_{h-1}^2=b_h(B_h+B_{h-1})$. Using $B_h+B_{h-1}=2B_h-b_h$, we find \[ \norm{\widetilde T_n-T_n}_{L^2}^2 =\sum_{h:\,b_h>0}b_h\Bigl(1-\sqrt{1-\frac{b_h}{2B_h}}\Bigr)^2 \le\sum_{h:\,b_h>0}\min\Bigl\{b_h,\frac{b_h^3}{4B_h^2}\Bigr\}, \] where we used $0\le1-\sqrt{1-x}\le x$ for $x\in[0,1]$. Fix $\varepsilon\in(0,1)$. The heights with $B_h<\varepsilon$ form an initial segment, on which $\sum b_h<\varepsilon$. On the heights with $B_h\ge\varepsilon$, we use the second term in the minimum and $\sum_hb_h=1$. We obtain \[ \norm{\widetilde T_n-T_n}_{L^2}^2\le\varepsilon+\frac{\bar b_n^2}{4\varepsilon^2} . \] By Step 1, the upper limit of the right side as $n\to\infty$ is $\varepsilon$, and letting $\varepsilon\downarrow0$ gives $\norm{\widetilde T_n-T_n}_{L^2}\to0$. \paragraph{Step 5: convergence to the universal kernel.} Let $x\in J_i$ and $y\in J_k$, with $h=\max(i,k)$. Then $\max(x,y)<\max(B_i,B_k)=B_h$, because $xB_{h-1}\ge B_h-\bar b_n$, and if $h=k$, the same holds for $y$. This gives \[ \max(x,y)\eta, \] since either $h_0=0$ and $c_{i3}\ge\kappa>\eta$, or $D_{i3,h_0-1}0\qquad\text{and}\qquad 1-\rho_{i3,H_i}\le\frac{2\Delta(v_i,v_3)}\eta\le2\eta . \end{equation} Indeed, if $1-\rho_{i3,h}>2\Delta(v_i,v_3)/\eta$ for every $h\ge h_0$ with $d_{i3,h}>0$, then \[ \Delta(v_i,v_3)\ge\sum_{h\ge h_0}d_{i3,h}(1-\rho_{i3,h})>\frac{2\Delta(v_i,v_3)}\eta\cdot\eta=2\Delta(v_i,v_3), \] which is impossible, since $\Delta(v_i,v_3)\ge0$. (The strict inequality holds because some $d_{i3,h}$ with $h\ge h_0$ is positive.) The second inequality in \eqref{eq:geometry-grade-choice} follows from $\Delta(v_i,v_3)\le\varepsilon=\eta^2$. This is the reason for the choice of $H_i$: the pair deficit is an average of $1-\rho_{i3,h}$ with weights $d_{i3,h}$, the alignment can fail only at heights where the cross mass is small, and the heights beyond $h_0$ carry cross mass at least $\eta$. Because $H_i\ge h_0$, we also have \begin{equation}\label{eq:geometry-grade-mass} D_{i3,H_i}\ge c_{i3}-\eta . \end{equation} \paragraph{Step 2: alignment on the prefix up to $H_i$.} Let $x_i=\Pi_{\le H_i}v_i$ and $z_i=\Pi_{\le H_i}v_3$, and write \[ \Gamma=D_{i3,H_i}=\ip{x_i}{z_i},\qquad X=B_{i,H_i}=\norm{x_i}^2,\qquad Z=B_{3,H_i}=\norm{z_i}^2 . \] By \eqref{eq:geometry-grade-mass}, we have $\Gamma\ge\kappa-\kappa/4=3\kappa/4$. Using $\Gamma\le\sqrt{XZ}$ and $X,Z\le1$, we find $X,Z\ge\Gamma^2\ge9\kappa^2/16$. The last increments $\xi=\norm{\Pi_{H_i}v_i}^2$, $\zeta=\norm{\Pi_{H_i}v_3}^2$, and $\gamma=d_{i3,H_i}$ satisfy $\xi,\zeta\le\bar b\le\varepsilon$ and $\gamma\ge0$, and \[ \rho_{i3,H_i}=\frac{\Gamma-\gamma/2}{\sqrt{(X-\xi/2)(Z-\zeta/2)}}\le\frac{\Gamma}{\sqrt{XZ}}\cdot\frac1{1-\sigma}, \qquad \sigma=\frac{8\varepsilon}{9\kappa^2}\le\frac1{18}, \] where we used $(X-\xi/2)/X\ge1-\sigma$, $(Z-\zeta/2)/Z\ge1-\sigma$, and $\varepsilon\le\kappa^2/16$. Using $\Gamma/\sqrt{XZ}\le1$ and $1/(1-\sigma)\le1+2\sigma$, we have $\rho_{i3,H_i}\le\Gamma/\sqrt{XZ}+2\sigma$. Combining this with \eqref{eq:geometry-grade-choice}, we obtain \[ 1-\frac{\Gamma}{\sqrt{XZ}}\le(1-\rho_{i3,H_i})+2\sigma\le2\eta+\frac{16\varepsilon}{9\kappa^2}\le\frac{4\eta}{\kappa^2} . \] Let $\alpha_i=\Gamma/Z$. Then \[ \norm{x_i-\alpha_iz_i}^2=X-\frac{\Gamma^2}Z=X\Bigl(1-\frac{\Gamma^2}{XZ}\Bigr)\le2\Bigl(1-\frac{\Gamma}{\sqrt{XZ}}\Bigr)\le\frac{8\eta}{\kappa^2}, \] and $\norm{\alpha_iz_i}=\Gamma/\sqrt Z\le\sqrt X\le1$. We have established that \begin{equation}\label{eq:geometry-prefix-alignment} x_i=\alpha_iz_i+e_i,\qquad \norm{e_i}\le\frac{2\sqrt2}{\kappa}\varepsilon^{1/4},\qquad\norm{\alpha_iz_i}\le1\qquad(i=1,2). \end{equation} \paragraph{Step 3: comparison on the shorter prefix.} By symmetry in the indices $1$ and $2$, we may assume that $H_1\le H_2$. Applying $\Pi_{\le H_1}$ to \eqref{eq:geometry-prefix-alignment} with $i=2$, and using $\Pi_{\le H_1}z_2=\Pi_{\le H_1}v_3=z_1$, we find $\Pi_{\le H_1}v_2=\alpha_2z_1+e_2'$ with $\norm{e_2'}\le\norm{e_2}$. Because the overlaps $d_{12,h}$ are all nonnegative, we have \[ c_{12}=\sum_hd_{12,h}\ge\sum_{h\le H_1}d_{12,h}=\ip{x_1}{\Pi_{\le H_1}v_2} =\ip{\alpha_1z_1+e_1}{\alpha_2z_1+e_2'} . \] We expand the last inner product. We have $\norm{\alpha_1z_1}\le1$, $\norm{\alpha_2z_1}\le\norm{\alpha_2z_2}\le1$, and $\norm{e_1}\le\norm{x_1}+\norm{\alpha_1z_1}\le2$. The three cross terms are therefore bounded in absolute value by $\norm{e_2'}+\norm{e_1}+2\norm{e_2'}\le(8\sqrt2/\kappa)\varepsilon^{1/4}$, and \[ c_{12}\ge\alpha_1\alpha_2B_{3,H_1}-\frac{8\sqrt2}{\kappa}\varepsilon^{1/4} . \] For the main term, we use \eqref{eq:geometry-grade-mass}, $B_{3,H_2}\le1$, and $c_{13},c_{23}\le1$: \[ \alpha_1\alpha_2B_{3,H_1}=D_{13,H_1}\frac{D_{23,H_2}}{B_{3,H_2}} \ge(c_{13}-\eta)(c_{23}-\eta)\ge c_{13}c_{23}-2\eta\ge c_{13}c_{23}-2\varepsilon^{1/4}. \] Combining the last two displays, we find \begin{equation}\label{eq:geometry-product-quantitative} c_{12}\ge c_{13}c_{23}-\frac{14}{\kappa}\varepsilon^{1/4} \qquad\text{whenever } c_{13},c_{23}\ge\kappa\text{ and }\varepsilon\le\frac{\kappa^2}{16} . \end{equation} \paragraph{Step 4: uniformity.} Let $\kappa\in(0,1]$, and let $\delta\le1$ be so small that $K_0\delta^{1/4}\le\kappa^2/16$. Let $v_1,v_2,v_3$ be an admissible triple with $\max_i\delta(v_i)\le\delta$. If $c_{13}<\kappa$ or $c_{23}<\kappa$, then $c_{13}c_{23}-c_{12}\le c_{13}c_{23}<\kappa$, because all overlaps lie in $[0,1]$. Otherwise, \eqref{eq:geometry-triple-epsilon} and \eqref{eq:geometry-product-quantitative} imply that $c_{13}c_{23}-c_{12}\le14\kappa^{-1}K_0^{1/4}\delta^{1/16}$. This shows that \[ \omega(\delta)\le\max\bigl\{\kappa,\,14\kappa^{-1}K_0^{1/4}\delta^{1/16}\bigr\}, \] and $\limsup_{\delta\downarrow0}\omega(\delta)\le\kappa$. Since $\kappa\in(0,1]$ is arbitrary, we conclude that $\omega(\delta)\to0$, as desired. \end{proof}