\chapter{Scalar response and stability}\label{sec:sc}\label{sec:scalar-stability} In this section, we study the scalar Parisi equation of a single spin under an arbitrary profile and the scalar response operator $J^{\scal}_{a,d}$ built from it. The cavity interpolation of \cref{sec:c7} decouples one spin from the others. At the independent endpoint of that interpolation, the decoupled spin follows the scalar law of \cref{sec:sc-law} with coefficient $d=\beta^2(1-t/N)$, and in \cref{sec:c7-endpoint}, we express the derivative of the cavity covariance at this endpoint through $J^{\scal}_{a,d}$, applied to the covariance of the rest self-overlap. The contraction argument of \cref{sec:c7-closure} needs the order bound $J^{\scal}_{a,d}\preceq(1+\varepsilon_N)I$ with $\varepsilon_N\le\rho/4$ at a minimizing profile. The goal of this section is to prove this bound with $\varepsilon_N\le C_{\rm st}[\rho^{-3/4}\eta^{1/4}+\lambda^2+N^{-1}]$, where $\eta$ is a trial budget (\cref{prop:lz-stability}). The argument has four steps. \begin{enumerate} \item We show in \cref{lem:sc-response} that, for every profile, $J_{a,d}$ is the derivative of the mean square magnetization $\Gamma_{a,d}$ when the covariance levels are transported by $q\mapsto q+\theta\varphi(q)$. \item The scalar Parisi functional is convex. We compare its second derivative along a transport of levels with the lower bound given by convexity and the first variation, and we find that $J^{\scal}_{a,d}$ is self-adjoint and that it is dominated by multiplication by the multiplier $k_{a,d}(q)=d\,\E^0h_q^2$, for every profile (\cref{lem:Jdom}). \item At the scalar Parisi measure, we have $k=1$ on $\supp\mu_\beta=[0,q_\beta]$ and $k(q)\le e^{-\beta^2(q-q_\beta)/2}$ above it (\cref{lem:reference}). On the support, this follows from an identity of Talagrand. Above the support, we use the log-concavity of a transformed density of the scalar diffusion and its heat evolution, both from \cite{Lopatto}. \item The multiplier depends Lipschitz continuously on the profile in $L^1$ and on $d$ (\cref{lem:scalarcontinuity}). By \cref{prop:loc-isolation}, a finite-dimensional minimizer is close in $L^1$ to the scalar trial profile, which is close to $\beta\alpha_\beta$. Combining these facts with the first three steps, we obtain \cref{prop:lz-stability}. \end{enumerate} The bound is marginal: at the Parisi measure, $k=1$ on the support, where the multiplier gives no contraction. The contraction in \cref{sec:c7-closure} comes instead from the factor $t=1-\rho$, and it needs only $\varepsilon_N\le\rho/4$. In the physics literature, De Dominicis and Kondor~\cite[pp.~606--608]{DeDominicisKondor1983} found that Parisi's solution with replica symmetry breaking is marginally stable in a truncated replica model near the critical temperature. The scalar identity on the support that expresses this marginality appears in \cite[Eqs.~(22)--(23)]{CrisantiRizzo2002}. Sommers and Dupont gave an earlier variational formulation of the coupled equations for the local magnetization and the distribution of frozen fields~\cite[Section~2, Eqs.~(1)--(7), and Eq.~(33)]{SommersDupont1984}; see also \cite[Section~III, (14)--(18), (22)--(23)]{CrisantiRizzo2002}. Those equations use the physical field and the order-parameter function $q(x)$. Here we use the covariance level $q$ and the integrated formulation in terms of probability measures described below. We use the following results from earlier sections: the generalized law and \cref{lem:fnd-posterior} of \cref{sec:gauss} for the basic properties of the scalar law, \cref{lem:fnd-path-heat} for the differentiation in \cref{lem:sc-response}, and, from \cref{sec:lz}, the trial budget \eqref{eq:loc-trialbudget}, the root growth \eqref{eq:lz-gsroot}, the description \eqref{eq:loc-scalar-measure} of $\mu_\beta$, and \cref{prop:loc-isolation}. The results of this section are used later as follows. The scalar law, described by \eqref{eq:sc-pde} and \eqref{eq:sc-joint-law}, and the kernel bounds of \cref{lem:cl-scalar} enter the cavity expansion in \cref{sec:c7,sec:c7-endpoint}. The operator \eqref{eq:scalarJexplicit} and its kernel form \eqref{eq:sc-kernel-form} are used in \cref{lem:linear}, \cref{lem:Jdom} in \cref{prop:c7-closure}, and \cref{prop:lz-stability} in the proof of \cref{thm:main} in \cref{sec:b7}. \paragraph{Standing assumptions and notation.} Throughout this section, $\beta>1$ is fixed and $d\in[\beta^2/2,\beta^2]$. A \emph{profile} is the distribution function $a(q)=\mu([0,q])$ of a Borel probability measure $\mu$ on $[0,1]$; it is nondecreasing and right-continuous, and $a(1)=1$. We write $\mu=s\delta_0+\nu$ with $s\ge0$, where the measure $\nu\ge0$ may charge $0$. The scalar law depends only on $a$. The decomposition enters only through $\nu$, which appears in the response operator. A \emph{step profile} is a profile with finitely many values. Integrals over $[0,q]$ include an atom at $q$, and integrals over $(q,1]$ exclude it. Unless stated otherwise, $C_\beta$ denotes a constant depending only on $\beta$, whose value may change from line to line. It does not depend on $d\in[\beta^2/2,\beta^2]$, on $s$, or on the profile, including the positions and masses of its atoms. No profile is assumed to minimize a functional until \cref{sec:sc-minimizer}. \section{The scalar law}\label{sec:sc-law} The scalar Parisi equation and its diffusion are \begin{equation}\label{eq:sc-pde} \begin{aligned} \partial_q u&=-\frac d2\bigl(\partial_{xx}u+a(q)(\partial_xu)^2\bigr), &u(1,x)&=\log(2\cosh x),\\ \dd Y_q&=d\,a(q)\partial_xu(q,Y_q)\dd q+\sqrt d\dd B_q, &Y_0&=0, \end{aligned} \end{equation} where $B$ is a standard Brownian motion. We write $u=u_{a,d}$ when the parameters need to be shown. Subscripts $x$ denote spatial derivatives, and $u_j=\partial_x^ju$. When $a=\alpha_\beta$ and $d=\beta^2$, the value $u(0,0)$ is the first term of the scalar Parisi functional \eqref{eq:intro-parisi} at its minimizer. \paragraph{Solutions and regularity.} For a step profile, \eqref{eq:sc-pde} has a classical solution on each interval where $a$ is constant. For a general profile, $u$ is the uniform limit of the solutions for step profiles whose measures converge weakly to $\mu$ \cite[Section~2.1]{Lopatto}. By \cite[Proposition~2.1]{Lopatto}, applied with $\beta^2$ replaced by $d$, the function $u(q,\cdot)$ is even, its spatial derivatives of every positive order are bounded and jointly continuous on $[0,1]\times\R$, and the spatial derivatives of the approximating solutions converge uniformly \cite[(2.2)]{Lopatto}. The terminal value in \cite{Lopatto} is $\log\cosh x$; it differs from ours by the constant $\log2$, which shifts $u$ by $\log2$ and does not change its spatial derivatives. The distribution functions of the approximating measures converge to $a$ at every continuity point of $a$, that is, at all but countably many points. Passing to the limit in the equations integrated in the level variable, we find that \begin{equation}\label{eq:sc-pde-integrated} u(q,x)-u(r,x)=\frac d2\int_q^r\bigl(u_{xx}+a\,u_x^2\bigr)(v,x)\dd v, \qquad 0\le q\le r\le1,\ x\in\R . \end{equation} In particular, $u$ is Lipschitz in $q$, since the integrand is bounded. For the weak space--time interpretation of the Parisi equation for general measures, see \cite[Theorem~4]{JagannathTobasco2016}. At an atom of $\mu$, the solution need not be differentiable in $q$. We read \eqref{eq:sc-pde} and every other parabolic equation in this section in this integrated form, including the linearized equations derived below, and we never differentiate $a$. \paragraph{Linear backward equations.} Several proofs below use linear equations of the form \begin{equation}\label{eq:sc-linear} \partial_qw+\frac{c(q)}2\,w_{xx}+b\,w_x+V\,w=-F, \end{equation} where $c$ is measurable with values in $[\beta^2/4,2\beta^2]$, and $b$, $V$, and $F$ are bounded functions of $(q,x)$ that are measurable in $q$ and have bounded continuous spatial derivatives. We use \eqref{eq:sc-linear} only for functions $w$ that are Lipschitz in $q$ and have bounded continuous spatial derivatives of every order. We read it in integrated form, as in \eqref{eq:sc-pde-integrated}. Fix $(q,x)$, and let $Z$ solve $\dd Z_r=b(r,Z_r)\dd r+\sqrt{c(r)}\dd B_r$ for $r\ge q$, with $Z_q=x$. Itô's formula applies to $r\mapsto e^{\int_q^rV(v,Z_v)\dd v}w(r,Z_r)$, with the derivative of $w$ in $q$ taken almost everywhere; to see this, one may mollify $w$ in the level variable and pass to the limit, using that the derivatives are bounded. Taking expectations, we obtain the Feynman--Kac representation \begin{equation}\label{eq:sc-backward} w(q,x)=\E\Bigl[e^{\int_q^1V(v,Z_v)\dd v}\,w(1,Z_1) +\int_q^1e^{\int_q^rV(v,Z_v)\dd v}F(r,Z_r)\dd r\Bigr]. \end{equation} In particular, if $w(1,\cdot)=0$, then $\sup_x|w(q,x)|\le e^{\|V\|_\infty}\int_q^1\sup_x|F(r,x)|\dd r$. \paragraph{Notation.} We write $\Pp^0$ and $\E^0$ for probability and expectation under the law of $Y$, together with a terminal spin $\epsilon\in\{-1,1\}$, which is sampled given $Y_1$ with \[ \Pp^0(\epsilon=\pm1\mid Y_1)=\frac{e^{\pm Y_1}}{2\cosh Y_1} =e^{\pm Y_1-u(1,Y_1)}. \] Let $\calG^0_q$ be the filtration of $Y$; the terminal spin is not $\calG^0_q$-measurable. We define \[ m_q=u_x(q,Y_q),\qquad h_q=u_{xx}(q,Y_q),\qquad \Gamma_{a,d}(q)=\E^0m_q^2,\qquad k_{a,d}(q)=d\,\E^0h_q^2 . \] We call $k_{a,d}$ the \emph{scalar multiplier}. For $0\le r\le\ell\le1$, let $P^0_{r,\ell}\psi(y)=\E^0[\psi(Y_\ell)\mid Y_r=y]$ be the transition operator of the Markov process $Y$, and set \[ f_p=m_p^2,\qquad \bar f_p=f_p-\E^0f_p,\qquad g_r^\ell(y)=P^0_{r,\ell}\bigl(u_x(\ell,\cdot)^2\bigr)(y), \] so that $g_r^\ell(Y_r)=\E^0[m_\ell^2\mid\calG_r^0]$. When we need the diffusion started from $y$ at level $r$, we write $Y^{r,y}$ and $\E_{r,y}$. \begin{lemma}[Basic properties of the scalar law]\label{lem:sc-basic} Let $a$ be a profile and $d\in[\beta^2/2,\beta^2]$. \begin{enumerate} \item[(a)] On $[0,1]\times\R$, we have \begin{equation}\label{eq:sc-basic-bounds} |\partial_xu|\le1,\qquad 0\le\partial_{xx}u\le1-(\partial_xu)^2\le1 . \end{equation} \item[(b)] For every $j\ge1$, there exists a constant $C_j(\beta)$, depending only on $\beta$ and $j$, such that $|u_j|\le C_j(\beta)$ on $[0,1]\times\R$. Further, $\sup_x|u_{xx}(q,x)-u_{xx}(r,x)|\le C_\beta|q-r|$ for all $q,r\in[0,1]$. \item[(c)] We have \begin{equation}\label{eq:sc-martingale} m_q=\E^0[\epsilon\mid\calG_q^0],\qquad m_0=0,\qquad \dd m_q=\sqrt d\,h_q\dd B_q,\qquad \Gamma_{a,d}'(q)=k_{a,d}(q). \end{equation} The function $k_{a,d}$ is continuous on $[0,1]$, and $\Gamma_{a,d}$ is continuously differentiable on $[0,1]$, with one-sided derivatives at the endpoints. \end{enumerate} \end{lemma} \begin{proof} We first identify the scalar law as a generalized law. We consider the generalized law of \cref{def:gauss-law} with $N=1$, $\Lambda=d$, all coupling coefficients equal to zero, root mass $s=0$, and the probability measure $\mu$ in place of $\nu$; this choice is allowed for every probability measure. The terminal value in \eqref{eq:fnd-general-pde} is then $\log\sum_{\sigma=\pm1}e^{x\sigma}=\log(2\cosh x)$, the Gaussian disorder does not enter, and the outer density is one. Hence the generalized law is the law of $(Y,\epsilon)$; it depends only on $a$. For one spin, the conditional covariance is $C_q=1-m_q^2$, and $H_q=h_q$. \Cref{lem:fnd-posterior} implies that $m_q=\E^0[\epsilon\mid\calG^0_q]$, that $m_0=0$, and that, for every $q\in[0,1]$, almost surely, \begin{equation}\label{eq:sc-posterior-as} a(q)\bigl(1-m_q^2\bigr)\le h_q\le1-m_q^2 . \end{equation} Differentiating \eqref{eq:sc-pde-integrated} in $x$, we see that $u_x$ satisfies the integrated form of $\partial_qu_x=-(d/2)(u_{xxx}+2a\,u_xu_{xx})$. Using Itô's formula along $Y$, we find that the drift terms cancel and that $\dd m_q=\sqrt d\,h_q\dd B_q$. This is the case $N=1$ of \eqref{eq:gauss-martingale}. \emph{Proof of (a).} Fix $q\in(0,1]$. Since the drift of $Y$ is bounded by $d$, Girsanov's theorem implies that the law of $Y_q$ is equivalent to the centered Gaussian law with variance $dq$. In particular, it charges every nonempty open interval. The functions \[ u_{xx}(q,\cdot)-a(q)\bigl(1-u_x(q,\cdot)^2\bigr),\qquad 1-u_x(q,\cdot)^2-u_{xx}(q,\cdot),\qquad 1-u_x(q,\cdot)^2 \] are continuous, and by \eqref{eq:sc-posterior-as} and $|m_q|\le1$, each of them is nonnegative at $Y_q$ almost surely. A continuous function with this property is nonnegative at every $x$. This proves \eqref{eq:sc-basic-bounds} for $q>0$, since $a(q)(1-u_x^2)\ge0$. Letting $q\downarrow0$ and using the joint continuity of $u_x$ and $u_{xx}$, we see that \eqref{eq:sc-basic-bounds} also holds at $q=0$. (With the right continuity of $a$, the lower bound $u_{xx}\ge a(q)(1-u_x^2)$ also holds everywhere.) \emph{Proof of (b).} We differentiate the equation and use the Feynman--Kac representation, following the method of \cite[Lemma~16]{JagannathTobasco2016}. By \eqref{eq:sc-basic-bounds}, we have $|u_1|\le1$ and $|u_2|\le1$. For $j\ge3$, the Leibniz rule gives \[ \partial_x^j(u_x^2)=2u_1u_{j+1}+2j\,u_2u_j +\sum_{i=2}^{j-2}\binom ji u_{i+1}u_{j-i+1}, \] with an empty sum for $j=3$. Differentiating \eqref{eq:sc-pde-integrated} $j$ times in $x$, we see that $u_j$ solves \eqref{eq:sc-linear} with \[ c=d,\qquad b=d\,a\,u_1,\qquad V=j\,d\,a\,u_2,\qquad F=\frac{d\,a}2\sum_{i=2}^{j-2}\binom ji u_{i+1}u_{j-i+1}, \] and terminal value $\partial_x^j\log(2\cosh x)$. Recall that the derivatives of $u$ are bounded by \cite[Proposition~2.1]{Lopatto}; in particular, the hypotheses of \eqref{eq:sc-backward} hold, with $Z=Y$. By \eqref{eq:sc-basic-bounds}, $V$ takes values in $[0,j\beta^2]$; note that the exponent in \eqref{eq:sc-backward} is nonnegative. Then \eqref{eq:sc-backward} implies that \[ \|u_j\|_\infty\le e^{j\beta^2}\Bigl( \|\partial_x^j\log(2\cosh x)\|_\infty +\frac{\beta^2}2\sum_{i=2}^{j-2}\binom ji \|u_{i+1}\|_\infty\|u_{j-i+1}\|_\infty\Bigr). \] Every derivative on the right has order between $3$ and $j-1$. By induction on $j$, we conclude that $\|u_j\|_\infty\le C_j(\beta)$ for all $j\ge1$, uniformly over profiles and $d\in[\beta^2/2,\beta^2]$. Differentiating \eqref{eq:sc-pde-integrated} twice in $x$, we find \[ u_{xx}(q,x)-u_{xx}(r,x)=\frac d2\int_q^r \Bigl[u_4+2a\bigl(u_2^2+u_1u_3\bigr)\Bigr](v,x)\dd v, \] and the integrand is bounded by a constant depending only on $\beta$. This proves the Lipschitz bound in (b). \emph{Proof of (c).} The first three identities in \eqref{eq:sc-martingale} were shown above. By Itô's isometry and $m_0=0$, we have \[ \Gamma_{a,d}(q)=\E^0m_q^2=d\int_0^q\E^0h_r^2\dd r =\int_0^qk_{a,d}(r)\dd r . \] By (b), we have $|h_q-h_r|\le C_\beta|q-r|+C_3(\beta)|Y_q-Y_r|$. Since $Y$ has continuous paths and $|h|\le1$, dominated convergence implies that $k_{a,d}$ is continuous. It follows that $\Gamma_{a,d}$ is continuously differentiable on $[0,1]$, with $\Gamma_{a,d}'=k_{a,d}$. \end{proof} We also use the exact path likelihood of the scalar law, for every profile, including profiles with atoms. It is the change of measure of \cite[Lemma~8.5 and Corollary~8.7]{JagannathTobasco2017PhaseDiagram}; we include the derivation in order to record the conventions at atoms. It extends the likelihood used for step profiles in the proof of \cref{lem:fnd-posterior} to every profile, without approximation. \begin{lemma}[Exact path likelihood]\label{lem:sc-likelihood} Let $a$ be a profile and $d\in[\beta^2/2,\beta^2]$. Under a reference law, let $X_q=\sqrt d\,B_q$, where $B$ is a standard Brownian motion. For every $q\in[0,1]$, the law of $(Y_r)_{0\le r\le q}$ has density \begin{equation}\label{eq:sc-prefix-law} \exp\Bigl\{a(q)u(q,X_q)-\int_{[0,q]}u(r,X_r)\,\mu(\dd r)\Bigr\} \end{equation} with respect to the law of $(X_r)_{0\le r\le q}$. The joint law of $(Y,\epsilon)$ has density \begin{equation}\label{eq:sc-joint-law} \exp\Bigl\{\epsilon X_1-su(0,0)-\int_{[0,1]}u(q,X_q)\,\nu(\dd q)\Bigr\} \end{equation} with respect to the product of the law of $X$ and counting measure on $\{-1,1\}$. The same holds if the coefficient $d$ in \eqref{eq:sc-pde} is replaced by a bounded measurable function $c(q)>0$ almost everywhere, and $X_q=\int_0^q\sqrt{c(r)}\dd B_r$. \end{lemma} \begin{proof} We write $\Upsilon_r=u(r,X_r)$. The drift $d\,a\,u_x$ of $Y$ is bounded, and by \eqref{eq:sc-basic-bounds}, we have \[ \exp\Bigl\{\frac d2\int_0^qa(r)^2u_x(r,X_r)^2\dd r\Bigr\}\le e^{\beta^2/2}, \] which is Novikov's condition. By Girsanov's theorem, the density of the law of $(Y_r)_{r\le q}$ with respect to the law of $(X_r)_{r\le q}$ is \[ \exp\Bigl\{\int_0^qa(r)u_x(r,X_r)\dd X_r -\frac d2\int_0^qa(r)^2u_x(r,X_r)^2\dd r\Bigr\}. \] Under the reference law, using Itô's formula and \eqref{eq:sc-pde-integrated}, we have \[ \dd\Upsilon_r=u_x(r,X_r)\dd X_r-\frac d2a(r)u_x(r,X_r)^2\dd r . \] The exponent therefore equals $\int_0^qa(r)\dd\Upsilon_r$. The function $a$ is right-continuous and of bounded variation, with $\dd a=\mu$ on $(0,1]$, and $\Upsilon$ is a continuous semimartingale. Integrating by parts, we have \[ a(q)\Upsilon_q-a(0)\Upsilon_0 =\int_{(0,q]}a(r-)\dd\Upsilon_r+\int_{(0,q]}\Upsilon_r\,\mu(\dd r). \] The functions $a(r-)$ and $a(r)$ differ only at the countably many atoms of $\mu$, which affects neither the stochastic integral nor the Lebesgue integral in $\dd\Upsilon_r$. Since $X_0=0$ and $a(0)=\mu(\{0\})$, we have $a(0)\Upsilon_0=\int_{\{0\}}u(r,X_r)\,\mu(\dd r)$. Inserting these facts into the previous display, we obtain \[ \int_0^qa(r)\dd\Upsilon_r=a(q)u(q,X_q)-\int_{[0,q]}u(r,X_r)\,\mu(\dd r). \] This proves \eqref{eq:sc-prefix-law}. At an atom of $\mu$ at $q$, the jump of the first term is canceled by the same atom in the integral, and at $q=0$ the density equals one. Given the path, the terminal spin has probability $e^{\epsilon Y_1-u(1,Y_1)}$ relative to counting measure. Multiplying \eqref{eq:sc-prefix-law} at $q=1$ by this factor, and using $a(1)=1$ and $\mu=s\delta_0+\nu$, we obtain \eqref{eq:sc-joint-law}. No further normalization is needed, since both factors are probability densities. For a coefficient $c(q)$ that is positive almost everywhere, we first choose the everywhere positive representative $c^+(q)=c(q)$ when $c(q)>0$ and $c^+(q)=1$ otherwise. It is measurable and bounded and equals $c$ almost everywhere. This change preserves every prefix clock, the integrated equation and drift, and the stochastic integral defining $X$. Thus the law and the likelihood are independent of this choice of representative. Let $C(q)=\int_0^qc(r)\dd r$. The substitution $\tau=C(q)/C(1)$ turns the equation with coefficient $c(q)$ into \eqref{eq:sc-pde} with coefficient $C(1)$ and the profile of the image of $\mu$ under $q\mapsto C(q)/C(1)$. This substitution is made in the integrated equation, using $\dd\tau=c(q)\dd q/C(1)$. Since $c>0$ almost everywhere, $q\mapsto C(q)/C(1)$ is an increasing homeomorphism of $[0,1]$; no positive lower bound on $c$ is required. By \cite[Proposition~2.1]{Lopatto}, applied with coefficient $C(1)$, the solution satisfies $|u_x|\le1$ and has bounded spatial derivatives. The argument above then applies with $d\dd r$ replaced by $c(r)\dd r$; in Novikov's condition, $\beta^2$ is replaced by an upper bound for $c$. \end{proof} \section{Continuity and kernel bounds} \label{sec:sc-kernels} The proof of the next lemma follows the comparison argument of \cite[Lemma~14]{JagannathTobasco2016}, which bounds the differences of the solutions and of their first spatial derivatives by the $L^1$ distance of the profiles. Here we also allow $d$ to vary and compare the second derivatives along the diffusion. \begin{lemma}[Continuity of the scalar multiplier]\label{lem:scalarcontinuity} There exists $C_\beta<\infty$ such that, for any two profiles $a,\widetilde a$ and any $d,\widetilde d\in[\beta^2/2,\beta^2]$, \begin{equation}\label{eq:scalarcontinuity} \sup_{0\le q\le1}|k_{a,d}(q)-k_{\widetilde a,\widetilde d}(q)| \le C_\beta\bigl(\|a-\widetilde a\|_{L^1(0,1)}+|d-\widetilde d|\bigr). \end{equation} \end{lemma} \begin{proof} Let $u$ and $\widetilde u$ solve \eqref{eq:sc-pde} for the two parameter pairs, and let $Y$ and $\widetilde Y$ be the corresponding diffusions. We set $\hat u=u-\widetilde u$ and $\Delta=\|a-\widetilde a\|_{L^1(0,1)}+|d-\widetilde d|$. The proof has three steps. We first bound $\hat u_x$ and $\hat u_{xx}$ by $C_\beta\Delta$, then couple the two diffusions, and finally compare the multipliers. \paragraph{Step 1: the difference of the solutions.} Subtracting the two equations and writing $u_x^2-\widetilde u_x^2=(u_x+\widetilde u_x)\hat u_x$, we find that $\hat u$ solves \eqref{eq:sc-linear} with \[ c=d,\qquad b=\omega,\qquad V=0,\qquad F=\Xi,\qquad \hat u(1,\cdot)=0, \] where \[ \omega=\frac{d\,a(q)}2\bigl(u_x+\widetilde u_x\bigr),\qquad \Xi=\frac{d-\widetilde d}2\,\widetilde u_{xx} +\delta(q)\,\widetilde u_x^2,\qquad \delta(q)=\frac{d\,a(q)-\widetilde d\,\widetilde a(q)}2 . \] Using \cref{lem:sc-basic}(a) and~(b), we see that $0\le\omega_x\le\beta^2$ and $|\omega_{xx}|\le C_\beta$. Further, \[ \Xi_x=\frac{d-\widetilde d}2\,\widetilde u_3 +2\delta\,\widetilde u_1\widetilde u_2,\qquad \Xi_{xx}=\frac{d-\widetilde d}2\,\widetilde u_4 +2\delta\bigl(\widetilde u_2^2+\widetilde u_1\widetilde u_3\bigr), \] and $2|\delta(q)|\le|d-\widetilde d|+\beta^2|a(q)-\widetilde a(q)|$. Using \cref{lem:sc-basic}(b) again, we find \[ \int_0^1\sup_x\bigl(|\Xi_x|+|\Xi_{xx}|\bigr)(q,x)\dd q \le C_\beta\int_0^1\bigl(|d-\widetilde d|+|a(q)-\widetilde a(q)|\bigr)\dd q \le C_\beta\Delta . \] Differentiating the equation for $\hat u$ once and twice in $x$, we see that $w_1=\hat u_x$ and $w_2=\hat u_{xx}$ solve \eqref{eq:sc-linear} with $c=d$, $b=\omega$, zero terminal values, and \[ V=\omega_x,\quad F=\Xi_x\qquad\text{and}\qquad V=2\omega_x,\quad F=\Xi_{xx}+\omega_{xx}w_1, \] respectively. Then \eqref{eq:sc-backward} implies that \[ \begin{aligned} \|w_1\|_\infty&\le e^{\beta^2}\int_0^1\|\Xi_x(q,\cdot)\|_\infty\dd q \le C_\beta\Delta,\\ \|w_2\|_\infty&\le e^{2\beta^2}\int_0^1\bigl(\|\Xi_{xx}(q,\cdot)\|_\infty +\|\omega_{xx}\|_\infty\|w_1\|_\infty\bigr)\dd q\le C_\beta\Delta . \end{aligned} \] This shows that \begin{equation}\label{eq:sc-pde-distance} \sup_{q,x}\bigl(|u_x-\widetilde u_x|+|u_{xx}-\widetilde u_{xx}|\bigr) \le C_\beta\Delta . \end{equation} \paragraph{Step 2: coupling the diffusions.} We drive $Y$ and $\widetilde Y$ by the same Brownian motion and set $D(q)=\sup_{r\le q}|Y_r-\widetilde Y_r|$. By \eqref{eq:sc-basic-bounds}, the drift $d\,a(r)u_x(r,\cdot)$ is $\beta^2$-Lipschitz in space, and at a common point it differs from $\widetilde d\,\widetilde a(r)\widetilde u_x(r,\cdot)$ by at most $|d-\widetilde d|+\beta^2|a(r)-\widetilde a(r)|+\beta^2C_\beta\Delta$, where we used \eqref{eq:sc-pde-distance}. Subtracting the integral equations for $Y$ and $\widetilde Y$, we obtain \[ D(q)\le\beta^2\int_0^qD(r)\dd r+C_\beta\Delta +|\sqrt d-\sqrt{\widetilde d}\,|\sup_{r\le1}|B_r| . \] Since $d,\widetilde d\ge\beta^2/2$, we have $|\sqrt d-\sqrt{\widetilde d}\,|\le|d-\widetilde d|/(\sqrt2\,\beta)$. By Gronwall's inequality and $\E\sup_{r\le1}|B_r|\le2$, we conclude that \begin{equation}\label{eq:sc-coupling} \E\sup_{q\le1}|Y_q-\widetilde Y_q| \le C_\beta\bigl(\Delta+|\sqrt d-\sqrt{\widetilde d}\,|\, \E\sup_{q\le1}|B_q|\bigr)\le C_\beta\Delta . \end{equation} The same argument, applied to the two diffusions started from a common point $y$ at a common level $r$, yields the same bound, uniformly in $(r,y)$. \paragraph{Step 3: the multipliers.} We write $h=u_{xx}(q,Y_q)$ and $\widetilde h=\widetilde u_{xx}(q,\widetilde Y_q)$. Note that $|h^2-\widetilde h^2|\le2|h-\widetilde h|$, because $0\le h,\widetilde h\le1$. Then \[ \begin{aligned} |k_{a,d}(q)-k_{\widetilde a,\widetilde d}(q)| &\le|d-\widetilde d|+2\beta^2\,\E|h-\widetilde h|\\ &\le|d-\widetilde d|+2\beta^2\Bigl(\|u_{xx}-\widetilde u_{xx}\|_\infty +\|u_3\|_\infty\,\E|Y_q-\widetilde Y_q|\Bigr). \end{aligned} \] Inserting \eqref{eq:sc-pde-distance}, \eqref{eq:sc-coupling}, and the bound $\|u_3\|_\infty\le C_3(\beta)$ into the last line, we obtain \eqref{eq:scalarcontinuity}. \end{proof} The next lemma collects the bounds on the kernels of the response operator that the cavity estimates of \cref{sec:c7-endpoint} use. Each bound retains a factor $\Gamma$ at the relevant levels. \begin{lemma}[Scalar kernels and their level weight]\label{lem:cl-scalar} For every profile $a$ and $d\in[\beta^2/2,\beta^2]$, write $\Gamma=\Gamma_{a,d}$. Then $\Gamma$ is nondecreasing and \begin{equation}\label{eq:cl-Gamma-bound} 0\le\Gamma(p)\le\min\{1,dp\}\le\min\{1,\beta^2p\}. \end{equation} For all $p,r,\ell\in[0,1]$, \begin{align} |\E^0[m_ph_pm_r]|&\le\sqrt{\Gamma(p)\Gamma(r)},& |\E^0[\bar f_p\epsilon m_r]|&\le\sqrt{\Gamma(p)\Gamma(r)}, \label{eq:cl-k1}\\ |\E^0[\bar f_pm_rm_\ell]|&\le\sqrt{\Gamma(p)\Gamma(r\wedge\ell)},& |\E^0[\bar f_pm_pm_r]|&\le\sqrt{\Gamma(p)\Gamma(p\wedge r)}, \label{eq:cl-k2}\\ 0\le\Var^0(f_p)&\le\Gamma(p),& 0\le\E^0[m_p^2h_p]&\le\Gamma(p). \label{eq:cl-k3} \end{align} For $\ell\ge p$, \begin{equation}\label{eq:cl-k4} |\Cov^0(f_p,g_p^\ell(Y_p))|\le\sqrt{\Gamma(p)\Gamma(\ell)}. \end{equation} \end{lemma} \begin{proof} By \cref{lem:sc-basic}(c) and \eqref{eq:sc-basic-bounds}, we have $\Gamma(p)=d\int_0^p\E^0h_r^2\dd r$, where $0\le h_r\le1$. This implies that $\Gamma$ is nondecreasing and that $0\le\Gamma(p)\le dp$. We also have $\Gamma\le1$, because $|m_p|\le1$. This proves \eqref{eq:cl-Gamma-bound}. Using $|m_p|\le1$ again, we have \[ \Var^0(f_p)=\E^0\bar f_p^2\le\E^0m_p^4\le\E^0m_p^2=\Gamma(p). \] The bounds below follow from the Cauchy--Schwarz inequality, together with $|h_p|\le1$, $|\epsilon|=1$, and $|m|\le1$: \[ \begin{aligned} |\E^0[m_ph_pm_r]|^2 &\le\E^0[m_p^2h_p^2]\,\E^0m_r^2\le\Gamma(p)\Gamma(r),\\ |\E^0[\bar f_p\epsilon m_r]|^2 &\le\E^0\bar f_p^2\,\E^0m_r^2\le\Gamma(p)\Gamma(r),\\ |\E^0[\bar f_pm_rm_\ell]|^2 &\le\E^0\bar f_p^2\,\E^0[m_r^2m_\ell^2]\le\Gamma(p)\Gamma(r\wedge\ell). \end{aligned} \] In the last line, we used $m_r^2m_\ell^2\le m_{r\wedge\ell}^2$, which holds because the factor at the smaller level is one of the two factors and the other is at most one. This proves \eqref{eq:cl-k1} and the first bound in \eqref{eq:cl-k2}; the second bound in \eqref{eq:cl-k2} is the case $\ell=p$. The bounds \eqref{eq:cl-k3} follow from the estimate on $\Var^0(f_p)$ and from $0\le h_p\le1$, which gives $0\le\E^0[m_p^2h_p]\le\E^0m_p^2$. Finally, let $\ell\ge p$. We have $0\le g_p^\ell\le1$ and $\E^0g_p^\ell(Y_p)=\E^0m_\ell^2=\Gamma(\ell)$, which imply that \[ \Var^0\bigl(g_p^\ell(Y_p)\bigr)\le\E^0\bigl(g_p^\ell(Y_p)\bigr)^2 \le\E^0g_p^\ell(Y_p)=\Gamma(\ell), \] and \eqref{eq:cl-k4} follows from the Cauchy--Schwarz inequality and the bound on $\Var^0(f_p)$. \end{proof} \section{The response operator}\label{sec:sc-response} For every profile, the operator defined below is the response of $\Gamma$ to a transport of covariance levels (\cref{lem:sc-response}). In \cite[Lemma~5.2, (H2)]{OpenAILimitingLaw}, a scalar response is written as a diagonal multiplier minus a positive semidefinite Hessian kernel. Here we identify the second variation of the scalar Parisi functional along transports of levels, and we compare it using the convexity of this functional along segments of distribution functions \cite{AuffingerChen2015Uniqueness}. In \cref{sec:sc-domination}, this shows that the scalar response operator is dominated by multiplication by $k_{a,d}$ at every profile. The transports fix the levels $0$ and $1$, and the operator acts on the \emph{scalar transport space} \[ \mathcal H_\nu=\bigl\{v\in L^2(\nu): v(0)=0\text{ if }\nu(\{0\})>0, \ v(1)=0\text{ if }\nu(\{1\})>0\bigr\}. \] This is a closed subspace of $L^2(\nu)$, and the orthogonal projection onto it is multiplication by $\ind_{(0,1)}$. The operator involves the derivative of $g_r^\ell$ in its argument. Since the noise of $Y$ is additive, the diffusion $Y^{r,y}$ started from $y$ at level $r$ solves an ordinary differential equation driven by the Brownian path, and it is differentiable in $y$. Its derivative is $\xi_\ell=\exp\{d\int_r^\ell a(v)u_{xx}(v,Y^{r,y}_v)\dd v\}$, which lies in $[1,e^{\beta^2}]$ by \eqref{eq:sc-basic-bounds}. Differentiating $g_r^\ell(y)=\E[u_x(\ell,Y^{r,y}_\ell)^2]$ under the expectation, we find \begin{equation}\label{eq:sc-dg} \partial_yg_r^\ell(y)=\E\bigl[2u_x(\ell,Y_\ell^{r,y}) u_{xx}(\ell,Y_\ell^{r,y})\,\xi_\ell\bigr],\qquad |\partial_yg_r^\ell|\le2e^{\beta^2}. \end{equation} \begin{definition}[Response operator]\label{def:sc-response} Let $a$ be a profile with $\mu=s\delta_0+\nu$, and let $d\in[\beta^2/2,\beta^2]$. For a bounded Borel function $\varphi$ on $[0,1]$ and $p\in[0,1]$, we define \begin{align} \frac1d(J_{a,d}\varphi)(p)={}& \E^0\bigl[h_p^2+2(1-a(p))m_p^2h_p\bigr]\varphi(p) -\int_{(p,1]}\E^0\bigl[m_p\partial_y g_p^\ell(Y_p)\bigr] \varphi(\ell)\,\nu(\dd\ell)\nonumber\\ &-2\int\E^0[m_ph_pm_r]\varphi(p\wedge r)\,\nu(\dd r) -\int\E^0[\bar f_p\epsilon m_r]\varphi(r)\,\nu(\dd r)\nonumber\\ &+\frac12\int a(r)\E^0[\bar f_pm_r^2]\varphi(r)\,\nu(\dd r) +\frac12\iint\E^0[\bar f_pm_rm_\ell]\varphi(r\wedge\ell) \,\nu(\dd r)\nu(\dd\ell)\nonumber\\ &+\frac12\int\nu(\dd r)\int_{(r,1]} \E^0\bigl[\bar f_pg_r^\ell(Y_r)\bigr]\varphi(\ell)\,\nu(\dd\ell). \label{eq:scalarJexplicit} \end{align} Integrals without a domain are over $[0,1]$. The same formula defines $J_{a,d}v$ for $v\in L^2(\nu)$. The \emph{scalar response operator} $J^{\scal}_{a,d}$ is the compression of $J_{a,d}$ to $\mathcal H_\nu$, that is, $J^{\scal}_{a,d}v=\ind_{(0,1)}J_{a,d}v$ for $v\in\mathcal H_\nu$. \end{definition} At an atom of $\nu$ at $p$, the right-continuous value $a(p)$ includes the atom, and the strict future interval $(p,1]$ excludes it. For $v\in L^2(\nu)$, the formula involves $v$ only through $v(p)$ and through values at points that are integrated against $\nu$, because $p\wedge r\in\{p,r\}$ and $r\wedge\ell\in\{r,\ell\}$. We show in the next paragraph that it defines $J_{a,d}v$ as an element of $L^2(\nu)$. \paragraph{Kernel form and boundedness.} We now rewrite \eqref{eq:scalarJexplicit}. For $r>p$, conditioning on $\calG^0_p$ and using \eqref{eq:sc-martingale}, we have $\E^0[m_ph_pm_r]=\E^0[m_p^2h_p]$, and $\nu((p,1])=1-a(p)$. Splitting the third term of \eqref{eq:scalarJexplicit} at $r=p$, we see that its part over $(p,1]$ equals $-2(1-a(p))\E^0[m_p^2h_p]\varphi(p)$, which cancels the second part of the first coefficient. In the double integral, we split $\varphi(r\wedge\ell)$ into the regions $r<\ell$, $\ellp\}}\E^0\bigl[m_p\partial_yg_p^r(Y_p)\bigr] -2\,\ind_{\{r\le p\}}\E^0[m_ph_pm_r] -\E^0[\bar f_p\epsilon m_r]\\ &+\frac12a(r)\E^0[\bar f_pm_r^2] +\int_{(r,1]}\E^0[\bar f_pm_rm_\ell]\,\nu(\dd\ell) +\frac12\nu(\{r\})\E^0[\bar f_pm_r^2]\\ &+\frac12\int_{[0,r)}\E^0\bigl[\bar f_pg_\ell^r(Y_\ell)\bigr]\,\nu(\dd\ell). \end{aligned} \end{equation} The term with $\nu(\{r\})$ is the diagonal part of the double integral. The kernel $\mathcal K_{a,d}$ is a bounded Borel function. Indeed, the first two terms are never both nonzero and are bounded by $2e^{\beta^2}$ by \eqref{eq:sc-dg}; since $|\bar f_p|\le1$, $|m|\le1$, and $0\le g\le1$, the third and fourth terms are bounded by $1$ and $1/2$, and the last three terms together by $\nu([0,1])\le1$. We conclude that $|\mathcal K_{a,d}|\le2e^{\beta^2}+3$. By the Cauchy--Schwarz inequality, $\|\int\mathcal K_{a,d}(\cdot,r)v(r)\,\nu(\dd r)\|_{L^2(\nu)} \le(2e^{\beta^2}+3)\nu([0,1])\|v\|_{L^2(\nu)}$. It follows that \eqref{eq:sc-kernel-form} extends to $v\in L^2(\nu)$, where it agrees with \eqref{eq:scalarJexplicit}. Using $0\le k_{a,d}\le d\le\beta^2$, we find $\|J_{a,d}\|_{L^2(\nu)\to L^2(\nu)}\le\beta^2(4+2e^{\beta^2})$. Compression does not increase the norm, which gives \begin{equation}\label{eq:sc-J-bounded} \|J^{\scal}_{a,d}\|_{\mathcal H_\nu\to\mathcal H_\nu}\le C_\beta . \end{equation} \paragraph{Transports of levels.} Let $\varphi$ be the restriction to $[0,1]$ of a smooth function, with $\varphi(0)=\varphi(1)=0$, and define $T_\theta(q)=q+\theta\varphi(q)$. We fix $\theta_0\in(0,1]$ such that $\theta_0\|\varphi'\|_\infty\le1/2$. For $|\theta|\le\theta_0$, the map $T_\theta$ is an increasing bijection of $[0,1]$ with $T_\theta'\in[1/2,3/2]$. We replace the covariance $d\,(q\wedge r)$ of $X$ in \eqref{eq:sc-joint-law} by $d\,T_\theta(q\wedge r)$ while keeping $\nu$. Equivalently, we replace the coefficient $d$ in \eqref{eq:sc-pde} by \[ c_\theta(q)=d\,T_\theta'(q)=d\bigl(1+\theta\varphi'(q)\bigr) \in\Bigl[\frac d2,\frac{3d}2\Bigr]\subset\Bigl[\frac{\beta^2}4,2\beta^2\Bigr], \] and keep $a$. We write $u_\theta$ and $Y^\theta$ for the resulting solution and diffusion, $u_{\theta,x}=\partial_xu_\theta$ and similarly for higher derivatives, and \[ \widetilde\Gamma_\theta(p)=\E\bigl[\partial_xu_\theta(p,Y^\theta_p)^2\bigr] \] for the resulting mean square magnetization. Let $a_\theta=a\circ T_\theta^{-1}$ be the distribution function of the image measure $T_{\theta\#}\mu$. Under the substitution $x'=T_\theta(q)$ in the level variable, the equation for $u_\theta$ becomes \eqref{eq:sc-pde} with coefficient $d$ and profile $a_\theta$, and the diffusion $Y^\theta$ becomes a time change of the diffusion for $a_\theta$. In formulas, \begin{equation}\label{eq:sc-transported} u_\theta(q,x)=u_{a_\theta,d}(T_\theta(q),x),\qquad \widetilde\Gamma_\theta(p)=\Gamma_{a_\theta,d}(T_\theta(p)), \end{equation} that is, $(u_\theta,Y^\theta)$ is the scalar law of $T_{\theta\#}\mu$ with coefficient $d$, observed at the transported levels. In particular, $\widetilde\Gamma_0=\Gamma_{a,d}$, and by \cref{lem:sc-basic}(b), the spatial derivatives of $u_\theta$ of each order are bounded uniformly in $|\theta|\le\theta_0$ and over profiles. \begin{lemma}[Response identity]\label{lem:sc-response} Let $a$ be a profile, let $d\in[\beta^2/2,\beta^2]$, and let $\varphi$ and $\widetilde\Gamma_\theta$ be as above. Then, for every $p\in[0,1]$, the function $\theta\mapsto\widetilde\Gamma_\theta(p)$ is continuously differentiable near $\theta=0$, and \[ \frac{\dd}{\dd\theta}\widetilde\Gamma_\theta(p)\Big|_{\theta=0} =(J_{a,d}\varphi)(p). \] \end{lemma} \begin{proof} The proof has four steps. In Step 1, we show that $u_\theta$ and its spatial derivatives are continuously differentiable in $\theta$; the argument works with the integrated equations and never differentiates $a$. In Step 2, we compute the parameter derivative of $u_\theta$ and prove \eqref{eq:scalarNodeVariation}. In Step 3, we write $\widetilde\Gamma_\theta(p)$ as a normalized expectation on a fixed Gaussian path space and differentiate it with \cref{lem:fnd-path-heat}. In Step 4, we match the resulting terms with those of \eqref{eq:scalarJexplicit}. Throughout the proof, $|\theta|\le\theta_0$, and constants may depend on $\beta$ and $\varphi$. \paragraph{Step 1: differentiability in the parameter.} Fix $\theta$, and for small $\delta\ne0$ let $v=u_{\theta+\delta}$, $u=u_\theta$, and $D_\delta=(v-u)/\delta$. Since $c_{\theta+\delta}-c_\theta=\delta d\varphi'$, subtracting the two equations and dividing by $\delta$, we find \begin{equation}\label{eq:sc-Dh} \partial_qD_\delta+\frac{c_\theta}2(D_\delta)_{xx} +\frac{c_\theta a}2(v_x+u_x)(D_\delta)_x =-\frac{d\varphi'}2\bigl(v_{xx}+a\,v_x^2\bigr),\qquad D_\delta(1,\cdot)=0 . \end{equation} This is \eqref{eq:sc-linear} with $c=c_\theta$, $V=0$, and a drift and a source whose spatial derivatives of each order are bounded uniformly in $\delta$ and $\theta$. Differentiating \eqref{eq:sc-Dh} $j$ times in $x$, we see that $\partial_x^jD_\delta$ solves an equation of the same form, with zeroth-order coefficient $j$ times the spatial derivative of the drift, and with a source that involves only derivatives of $D_\delta$ of order less than $j$ and spatial derivatives of the drift and of the source of \eqref{eq:sc-Dh}. By \eqref{eq:sc-backward} and induction on $j$, we have $\sup_{q,x}|\partial_x^jD_\delta|\le C_j$ for every $j\ge0$, uniformly in $\delta$ and $\theta$. In particular, $v-u=\delta D_\delta$ and all its spatial derivatives are $O(|\delta|)$. Next, we write the drift in \eqref{eq:sc-Dh} as $c_\theta a\,u_x+(c_\theta a/2)(v_x-u_x)$ and move the second part to the right side. For two increments $\delta$ and $\delta'$, the difference $D_\delta-D_{\delta'}$ then solves \eqref{eq:sc-linear} with drift $c_\theta a\,u_x$, $V=0$, zero terminal value, and the source \[ \frac{d\varphi'}2\Bigl[(v-v')_{xx}+a\bigl(v_x^2-v_x'^2\bigr)\Bigr] +\frac{c_\theta a}2\Bigl[(v_x-u_x)(D_\delta)_x-(v'_x-u_x)(D_{\delta'})_x\Bigr], \] where $v'=u_{\theta+\delta'}$. By the bounds just proved, every spatial derivative of this source is bounded by $C_j(|\delta|+|\delta'|)$. By the same induction, we have $\sup_{q,x}|\partial_x^j(D_\delta-D_{\delta'})|\le C_j(|\delta|+|\delta'|)$. It follows that, as $\delta\to0$, the functions $D_\delta$ converge uniformly, together with all their spatial derivatives, to a function $\dot u_\theta$. Passing to the limit in the integrated form of \eqref{eq:sc-Dh}, we find that $\dot u_\theta$ solves \begin{equation}\label{eq:sc-W} \partial_q\dot u_\theta+\frac{c_\theta}2(\dot u_\theta)_{xx} +c_\theta a\,u_{\theta,x}(\dot u_\theta)_x =-\frac{d\varphi'}2\bigl(u_{\theta,xx}+a\,u_{\theta,x}^2\bigr), \qquad \dot u_\theta(1,\cdot)=0 . \end{equation} We conclude that $u_\theta$ and each of its spatial derivatives are differentiable in $\theta$, with $\partial_\theta\partial_x^ju_\theta=\partial_x^j\dot u_\theta$, and that these derivatives are bounded uniformly in $(q,x)$ and $\theta$. To prove that these derivatives depend continuously on $\theta$, we set $b_\theta=c_\theta a\,u_{\theta,x}$, $F_\theta=(d\varphi'/2)(u_{\theta,xx}+a\,u_{\theta,x}^2)$, and $R=\dot u_\theta-\dot u_{\theta'}$. Subtracting \eqref{eq:sc-W} at the two parameters, we obtain \[ \Bigl(\partial_q+\frac{c_\theta}2\partial_{xx}+b_\theta\partial_x\Bigr)R =-(F_\theta-F_{\theta'}) -\frac{c_\theta-c_{\theta'}}2(\dot u_{\theta'})_{xx} -(b_\theta-b_{\theta'})(\dot u_{\theta'})_x, \qquad R(1,\cdot)=0 . \] Since $c_\theta-c_{\theta'}=(\theta-\theta')d\varphi'$, and since $u_\theta-u_{\theta'}$ and all its spatial derivatives are $O(|\theta-\theta'|)$ by the bound on $\partial_\theta\partial_x^ju_\theta$, every fixed-order spatial derivative of the right side is $O(|\theta-\theta'|)$. Using the same backward estimates, we have $\sup_{q,x}|\partial_x^jR|\le C_j|\theta-\theta'|$, so $\partial_x^j\dot u_\theta$ depends continuously on $\theta$, uniformly in $(q,x)$. The same argument applies without change to transports $q\mapsto q+\theta_1\varphi_1(q)+\theta_2\varphi_2(q)$ with several parameters, and gives continuous partial derivatives in each parameter. \paragraph{Step 2: the variation of the solution.} We write $\dot u=\dot u_0$ for the derivative at $\theta=0$. By \eqref{eq:sc-W} and \eqref{eq:sc-backward}, with $Z=Y$, we have \begin{equation}\label{eq:sc-udot-rep} \dot u(q,y)=\frac d2\int_q^1\varphi'(r)\Psi_q(r;y)\dd r,\qquad \Psi_q(r;y)=\E_{q,y}\bigl[h_r+a(r)m_r^2\bigr], \end{equation} where $\E_{q,y}$ refers to the diffusion started from $y$ at level $q$. To evaluate $\Psi_q(r;y)$, we use Itô's formula along $Y$. Differentiating \eqref{eq:sc-pde-integrated} twice in $x$ and using Itô's formula for $u_{xx}(r,Y_r)$, we find \[ \dd h_r=-d\,a(r)h_r^2\dd r+\sqrt d\,u_{xxx}(r,Y_r)\dd B_r, \] and by \eqref{eq:sc-martingale}, $\dd(m_r^2)=d\,h_r^2\dd r+2\sqrt d\,m_rh_r\dd B_r$. The product rule for the continuous semimartingale $m_r^2$ and the deterministic function $a$ of bounded variation gives $\dd(a(r)m_r^2)=a(r-)\dd(m_r^2)+m_r^2\,\mu(\dd r)$ on $(0,1]$, and $a(r-)=a(r)$ except at countably many $r$. Adding the two differentials, we see that the drift terms $\mp d\,a(r)h_r^2\dd r$ cancel, and \[ \dd\bigl(h_r+a(r)m_r^2\bigr) =\sqrt d\bigl[u_{xxx}(r,Y_r)+2a(r)m_rh_r\bigr]\dd B_r+m_r^2\,\mu(\dd r). \] Taking conditional expectations given $Y_q=y$, and recalling that $\mu=\nu$ on $(q,r]\subset(0,1]$, we obtain \begin{equation}\label{eq:sc-Fq} \Psi_q(r;y)-\Psi_q(q;y)=\int_{(q,r]}g_q^v(y)\,\nu(\dd v),\qquad q\le r\le1, \end{equation} where $\Psi_q(q;y)=u_{xx}(q,y)+a(q)u_x(q,y)^2$. We insert \eqref{eq:sc-Fq} into \eqref{eq:sc-udot-rep} and exchange the order of integration over $q0,\qquad V_q(-x)=V_q(x),\qquad x\in\R . \] Note that $V_q'(0)=0$ by evenness. Then $V_q'(x)\ge x/(dq)>0$ for $x>0$. This implies that $z_q$ is even, log-concave, and decreasing on $(0,\infty)$. We use this at $q=q_\beta$, where the right-continuous value is $a(q_\beta)=1$, including the atom of $\mu_\beta$ at $q_\beta$; in particular, $z_{q_\beta}=\pi_{q_\beta}e^{-u(q_\beta,\cdot)}$. \paragraph{Step 3: heat evolution above the support.} On $[q_\beta,1]$, we have $a=1$, and the solution of \eqref{eq:sc-pde} is \[ u(q,x)=\log(2\cosh x)+\frac{d(1-q)}2,\qquad q_\beta\le q\le1, \] by \cite[Lemma~2.4(i)]{Lopatto}; this formula can also be checked by direct substitution, since $u_x=\tanh x$, $u_{xx}=\sech^2x$, $u_{xx}+u_x^2=1$, and $\partial_qu=-d/2$. We write $G_v$ for the centered Gaussian density with variance $v$. By \cite[Lemma~2.4(ii)]{Lopatto}, applied with mass $m=1$ on $[q_\beta,1)$, we have, for $q_\betat\}+y)\cap\{g>t'\}\bigr|\dd t\dd t', \] where $|\cdot|$ is Lebesgue measure. The superlevel sets $\{f>t\}$ and $\{g>t'\}$ are open intervals centered at $0$. For two centered intervals $I$ and $I'$, we have $|(I+y)\cap I'|\le\min\{|I|,|I'|\}=|I\cap I'|$, and \eqref{eq:sc-rearrangement} follows. We use \eqref{eq:sc-rearrangement} with $f=z_{q_\beta}$ and $g=\sech^3$, which satisfy its hypotheses by Step 2. All the integrals below are finite, since $\sech\le1$ and $\int z_{q_\beta}=\E[e^{-u(q_\beta,Y_{q_\beta})}]\le1/2$. By \eqref{eq:sc-heat} and Tonelli's theorem, for $q_\beta0$ depending only on $\beta$. We claim that, for every $\lambda>0$, \begin{equation}\label{eq:sc-floor} \|\gamma^{\rm tr}_\lambda-\gamma_\beta\|_{L^1(0,1)} \le C_\beta\lambda^2 . \end{equation} Indeed, $\gamma^{\rm tr}_\lambda-\gamma_\beta=(\lambda-\gamma_\beta)_+$. Suppose first that $\lambda\le k_0T_0$. For $q\ge T_0$, since $\gamma_\beta$ is nondecreasing, we have $\gamma_\beta(q)\ge\gamma_\beta(T_0)\ge k_0T_0\ge\lambda$, and the difference vanishes there. This gives \[ \|\gamma^{\rm tr}_\lambda-\gamma_\beta\|_{L^1(0,1)} =\int_0^{T_0}(\lambda-\gamma_\beta(q))_+\dd q \le\int_0^{\lambda/k_0}(\lambda-k_0q)\dd q=\frac{\lambda^2}{2k_0}. \] If $\lambda>k_0T_0$, the difference is at most $\lambda$ everywhere, and $\lambda\le\lambda^2/(k_0T_0)$. Since $T_0\le1/4<2$, both cases give \eqref{eq:sc-floor} with $C_\beta=1/(k_0T_0)$. \begin{proposition}[Scalar stability at the minimizing profile] \label{prop:lz-stability} There exists a constant $C_{\rm st}\ge1$, depending only on $\beta$ (in particular, not on the minimizer or its atoms), with the following property. Let $N\ge2$, $0<\rho\le1$, $t=1-\rho$, and $0<\lambda\le\lambda_0$, and set $s=\lambda/\beta$. Let $\mu_N=s\delta_0+\nu_N$ be a minimizer of $\mathcal F_{t,s}$ in \eqref{eq:fnd-functional}, let $a_N(q)=\mu_N([0,q])$ be its profile, and let $\eta$ be a trial budget for the minimizer $\beta a_N$ of $F_\rho$, in the sense of \eqref{eq:loc-trialbudget}. Let $d_N=\beta^2(1-t/N)$. Then \begin{equation}\label{eq:lz-profileconvergence} \|a_N-\alpha_\beta\|_{L^1(0,1)} \le\min\bigl\{1,C_{\rm st}[\rho^{-3/4}\eta^{1/4}+\lambda^2]\bigr\}. \end{equation} Further, let $\varepsilon_N=\max\{0,\sup_{q\in[0,1]}k_{a_N,d_N}(q)-1\}$. Then, on the scalar transport space $\mathcal H_{\nu_N}$ of $\mu_N$, \begin{equation}\label{eq:lz-stability} J^{\scal}_{a_N,d_N}\preceq(1+\varepsilon_N)I, \qquad \varepsilon_N\le C_{\rm st} \bigl[\rho^{-3/4}\eta^{1/4}+\lambda^2+N^{-1}\bigr]. \end{equation} \end{proposition} \begin{proof} We use the energy normalization of \cref{sec:fnd}, in which $\gamma=\beta a$ and $F_\rho(\gamma)=\beta^{-1}\mathcal F_{t,s}(\mu)$. The map $\mu\mapsto\beta a$ is a bijection onto the admissible profiles of \cref{sec:lz}, and multiplication by $\beta^{-1}$ preserves minimizers. Hence $\gamma_N=\beta a_N$ is a minimizer of $F_\rho$, and $\eta$ is a trial budget for it. The hypotheses of \cref{prop:loc-isolation} hold, and \eqref{eq:loc-isolation} implies that $\|\gamma_N-\gamma^{\rm tr}_\lambda\|_{L^1}\le C\rho^{-3/4}\eta^{1/4}$, with a constant $C$ depending only on $\beta$. Using the triangle inequality and \eqref{eq:sc-floor}, we have \[ \|a_N-\alpha_\beta\|_{L^1} \le\beta^{-1}\bigl(\|\gamma_N-\gamma^{\rm tr}_\lambda\|_{L^1} +\|\gamma^{\rm tr}_\lambda-\gamma_\beta\|_{L^1}\bigr) \le C_\beta[\rho^{-3/4}\eta^{1/4}+\lambda^2]. \] The distance is also at most one, since both functions take values in $[0,1]$. This proves \eqref{eq:lz-profileconvergence}. Since $N\ge2$ and $0\le t<1$, we have $d_N\in[\beta^2/2,\beta^2]$ and $|d_N-\beta^2|=\beta^2t/N\le\beta^2/N$. Then \cref{lem:scalarcontinuity}, applied with $(a,d)=(a_N,d_N)$ and $(\widetilde a,\widetilde d)=(\alpha_\beta,\beta^2)$, and \cref{lem:reference} imply that, for every $q\in[0,1]$, whether or not $q$ lies in $\supp\mu_\beta$, \[ k_{a_N,d_N}(q)\le k_{\alpha_\beta,\beta^2}(q) +C_\beta\bigl(\|a_N-\alpha_\beta\|_{L^1}+N^{-1}\bigr) \le1+C_\beta\bigl(\|a_N-\alpha_\beta\|_{L^1}+N^{-1}\bigr). \] Together with \eqref{eq:lz-profileconvergence}, this yields the bound on $\varepsilon_N$ in \eqref{eq:lz-stability}. Finally, since $k_{a_N,d_N}\le1+\varepsilon_N$ pointwise, \cref{lem:Jdom}, applied to the profile $a_N$ with $\nu=\nu_N$, implies that $J^{\scal}_{a_N,d_N}\preceq M_{k_{a_N,d_N}}\preceq(1+\varepsilon_N)I$ on $\mathcal H_{\nu_N}$. Note that only the multipliers of the two profiles are compared; the operator inequality is proved on the transport space of the minimizer itself. We choose $C_{\rm st}\ge1$ larger than the constants in the two bounds; it depends only on $\beta$. \end{proof}