\documentclass[11pt]{article} \usepackage[T1]{fontenc} \usepackage[utf8]{inputenc} \usepackage{lmodern} \usepackage[margin=1in]{geometry} \usepackage{amsmath,amssymb,amsthm,mathtools,microtype,booktabs} \usepackage[hidelinks]{hyperref} \hypersetup{pdftitle={Centroid-body fixed points and boundary reciprocity},pdfauthor={Sihan Chen}} \setlength{\emergencystretch}{2em} \numberwithin{equation}{section} \newtheorem{theorem}{Theorem}[section] \newtheorem{proposition}[theorem]{Proposition} \newtheorem{lemma}[theorem]{Lemma} \newtheorem{corollary}[theorem]{Corollary} \theoremstyle{remark} \newtheorem{remark}[theorem]{Remark} \newcommand{\R}{\mathbb R} \newcommand{\Sn}{\mathbb S^{n-1}} \newcommand{\E}{\mathbb E} \newcommand{\dd}{\,\mathrm d} \newcommand{\Id}{\mathrm{Id}} \newcommand{\ip}[2]{\langle #1,#2\rangle} \DeclareMathOperator{\Aut}{Aut} \DeclareMathOperator{\Cov}{Cov} \DeclareMathOperator{\tr}{tr} \DeclareMathOperator{\sgn}{sgn} \newcommand{\C}{\mathcal C} \newcommand{\T}{\mathcal T} \newcommand{\norm}[1]{\left\lVert #1\right\rVert} \DeclareMathOperator{\Var}{Var} \title{Centroid-body fixed points\\and boundary reciprocity} \author{Sihan Chen} \date{November 2026} \begin{document} \maketitle \begin{abstract} We prove that, in every dimension, a convex body equal to a dilate of its classical volume-normalized centroid body is a centered ellipsoid. We place the argument in a general framework of affine spectra and boundary reciprocity. For every regular convex body and every positive moment exponent, a natural boundary Markov chain is reversible if and only if the body is a centered ellipsoid. Independently, an exact quadratic identity measures the failure of reciprocity of the map $u\mapsto h(u)\nabla h(u)$; it yields a sharp estimate for approximation of the squared support function by an ellipsoidal quadratic form. Affine covariance supplies universal eigenspaces for all $L_s$ centroid fixed-point equations, and quadratic orthogonality converts kernel approximation into a symmetry certificate. These structural results are proved without assuming the fixed-point classification. The classification itself still uses a signed moment gap in dimensions two through twenty-five and symmetry, curvature, and regression estimates in higher dimensions. All constants and finite certificates are included. No unproved reversibility assertion is used in that proof. \end{abstract} \noindent\textit{2020 Mathematics Subject Classification.} 52A20, 52A40, 60E15. \par\noindent\textit{Keywords.} Centroid body, fixed point, ellipsoid, boundary Markov chain, reversibility, compact transformation group, linear regression. \tableofcontents \section{Introduction and main theorem} For a convex body $K\subset\R^n$ with nonempty interior, define \begin{equation}\label{eq:centroid} h_{\Gamma K}(u)=\frac1{|K|}\int_K|\ip ux|\dd x. \end{equation} Here $\Gamma$ is the ordinary centroid operator: no polar or projection operator is composed with it. Throughout, centered means centered at the origin. Write $\kappa_j=|B_2^j|$, with $\kappa_0=1$, and set \[ a_n=\frac{2\kappa_{n-1}}{(n+1)\kappa_n}. \] Thus $\Gamma B_2^n=a_nB_2^n$. We also write $\T K=a_n^{-1}\Gamma K$. We study the equation \begin{equation}\label{eq:fixed} \Gamma K=cK,\qquad c>0. \end{equation} It implies that $K$ is origin symmetric. \begin{theorem}\label{thm:classification} Let $n\ge1$. A convex body $K\subset\R^n$ satisfies \eqref{eq:fixed} if and only if it is a centered ellipsoid. In that case $c=a_n$. \end{theorem} The higher-dimensional fixed-point question is stated as Problem~1 in Reuter~\cite{Reuter}, who proves classification in a Banach--Mazur neighborhood of the ellipsoids. The planar case is classical; see Petty~\cite{PettyPlane} and the discussion in \cite{Reuter}. Section~\ref{sec:finite} includes an independent proof of that case. Related fixed-point theorems for intersection bodies and polar centroid compositions are proved by Milman--Shabelman--Yehudayoff~\cite{MSY}. Their equations involve different operators. Our equation is for the volume-normalized ordinary centroid operator \eqref{eq:centroid} itself. The structural results are independent of this classification. Theorem~\ref{str:reversibility} characterizes ellipsoids by reversibility of a boundary moment chain, for every exponent $s>0$. Theorem~\ref{str:quadraticidentity} gives an exact identity for the reciprocity defect and the sharp estimate \[ \|h_L^2-h_{E_L}^2\|_{L^2(\sigma)}^2 \le\frac{n}{2(n+3)}\mathfrak R(L). \] The approximating quadratic form is positive definite, so $E_L$ is an actual ellipsoid. Theorem~\ref{str:affineidentity} and Corollary~\ref{str:spectralcertificate} explain why affine deformations, moment cancellation, and quadratic regression govern the fixed-point problem. A direct passage from the fixed-point equation to reciprocity would shorten the proof, but that passage is not established independently here; the estimates below remain part of the classification argument. Here is the organization of the classification proof, following the structural results in Sections~\ref{sec:reciprocity} and~\ref{sec:affinestructure}. \begin{enumerate} \item In dimensions $2\le n\le25$, a signed cosine-transform energy estimate forces the radial function to be constant in inertia position. \item In dimensions $n\ge26$, affine eigenfunctions of a boundary integral operator and their quadratic orthogonality force a large automorphism group. Compact-group dimension estimates and reflection rigidity yield a canonical independent rotation subspace of dimension \[ p\ge\lceil2n/3\rceil,\qquad p\ge19\quad\hbox{if }n=27. \] The extra restriction at $n=27$ uses a nine-dimensional representation argument. \item An explicit curvature bound for squared centroid support norms, a regression estimate with constant $1/14$, and a weighted radial moment bound give a necessary inequality for every proper invariant rotation subspace. It contradicts the preceding dimension bound. A uniform comparison treats $n\ge32$; six rational comparisons treat $26\le n\le31$. \end{enumerate} The analytic constants are \[ \gamma=\frac{77\,6^{4/3}}{4800}>\frac{87}{500}, \qquad \inf_{\lambda}\E(g(Z)-\lambda Z)^2\le\frac{L^2}{14}\E Z^2, \] where the second assertion holds for increasing concave $L$-Lipschitz $g$ with $g(0)=0$ and positive $Z$ with log-concave survival. The precise hypotheses and proofs appear below. The external inputs are stated at their points of use: the Busemann--Petty centroid inequality, Berwald's inequality, log-concavity of marginals, Ball's convexity theorem, the normalized Mellin moment theorem, the classical maximal-subgroup classification, and the positive compact-operator theorem. The spherical and cone measures are normalized separately; throughout, spherical integration is with probability measure. For standard convex-geometric notation we refer to \cite{Schneider}. \section{Normalization and one-dimensional moment bounds} Change of variables gives \begin{equation}\label{eq:equivariance} \Gamma(AK)=A\Gamma K\qquad(A\in GL(n,\R)). \end{equation} We may therefore put a fixed body in inertia position. If $U$ is uniform in $K$, this means \begin{equation}\label{eq:inertia} \Cov(U)=\tau\Id,\qquad \tau>0. \end{equation} Every linear automorphism is then orthogonal. We write \[ G=\Aut(K):=\{A\in GL(n,\R):AK=K\},\qquad d=\dim G,\qquad V=|K|. \] Thus $G$ is a closed compact group, including all its components; $G^0$ denotes its identity component. The Busemann--Petty centroid inequality \cite{Petty,BB} gives \begin{equation}\label{pre:BP} |\Gamma K|\ge a_n^n|K|,\qquad\hbox{hence }c\ge a_n. \end{equation} \begin{lemma}\label{pre:moments} For a uniformly distributed point $X$ in a symmetric convex body, \begin{equation}\label{pre:momentbounds} \sqrt{\frac{n+2}{2(n+1)}}\, (\E\ip uX^2)^{1/2} \le\E|\ip uX| \le\frac{\sqrt3}{2}(\E\ip uX^2)^{1/2}. \end{equation} Consequently a fixed body in inertia position has radial ratio at most \begin{equation}\label{pre:radialratio} Q_n=\sqrt{\frac{3(n+1)}{2(n+2)}}. \end{equation} \end{lemma} \begin{proof} On $K_+=K\cap\{\ip ux\ge0\}$, apply Berwald's inequality \cite{Berwald,LP} to the nonnegative affine function $x\mapsto\ip ux$ at exponents one and two. Symmetry yields \[ \left(\frac{(n+1)(n+2)}2\E\ip uX^2\right)^{1/2} \le(n+1)\E|\ip uX|. \] For the upper bound, the density of $Y=\ip uX$ is even and nonincreasing on the positive half-line by Brunn's section concavity theorem. Layer cake expresses it as a probability mixture of uniform laws on $[-S,S]$. Hence $\E|Y|=\E S/2$ and $\E Y^2=\E S^2/3\ge(\E S)^2/3$. For a fixed body, \eqref{pre:momentbounds} bounds its support function between $\sqrt{\tau(n+2)/(2(n+1))}/c$ and $\sqrt{3\tau}/(2c)$. The minimum and maximum of the support function are the inradius and circumradius, respectively, as are the corresponding radial extrema. Their quotient gives \eqref{pre:radialratio}. \end{proof} \section{Boundary reciprocity and ellipsoids}\label{sec:reciprocity} This section does not assume the fixed-point equation. Let $n\ge2$ and let $L$ be a convex body containing the origin in its interior, with $C^2$ support function $h_L$ and positive tangential Hessian. Extend $h_L$ one-homogeneously away from the origin, and write $\sigma$ for spherical probability measure. Put \[ x_L(u)=\nabla h_L(u),\qquad \mu_L(\dd u)=\frac{h_L(u)}{n|L|}S_L(\dd u). \] In particular, $\mu_L$ is a probability measure with continuous positive density. It is useful to allow nonsymmetric $L$ here. Fixed bodies in the main theorem satisfy this regularity, as proved in Section~\ref{sec:boundary}. \subsection{The boundary moment chain} For $s>0$ define \begin{align} m_{L,s}(u)&=\int|\ip u{x_L(v)}|^s\mu_L(\dd v),\notag\\ p_{L,s}(u,v)&=\frac{|\ip u{x_L(v)}|^s}{m_{L,s}(u)},\qquad P_{L,s}f(u)=\int p_{L,s}(u,v)f(v)\mu_L(\dd v). \label{str:chain} \end{align} This is a Markov operator. If $U_L$ is uniform in $L$, radial integration gives the normalization \begin{equation}\label{str:chainnormalization} m_{L,s}(u)=\frac{n+s}{n}\E|\ip u{U_L}|^s. \end{equation} For $s=1$ and $\Gamma L=cL$, this is exactly the operator $Q$ used in the classification argument below. \begin{lemma}\label{str:stationary} The kernel of $P_{L,s}^2$ is continuous and strictly positive on $\Sn\times\Sn$. Consequently $P_{L,s}$ has a unique stationary probability $\pi_{L,s}=w_{L,s}\mu_L$, where $w_{L,s}$ is continuous and strictly positive. \end{lemma} \begin{proof} All the kernels and denominators in \eqref{str:chain} are continuous, and the denominators are positive. For fixed $u,v$, the two functions $w\mapsto|\ip u{x_L(w)}|$ and $w\mapsto|\ip w{x_L(v)}|$ have zero sets with empty interior. For the first this follows from strict convexity: an open boundary patch cannot lie in a hyperplane; for the second it is immediate. Their positive sets are open and dense. Their intersection therefore contains an open set of positive $\mu_L$ measure, proving strict positivity of the two-step kernel. Compactness gives a lower bound $\delta>0$ for that kernel. A continuous Markov kernel on a compact space has a stationary probability: take a weak limit of the Ces\`aro averages of the laws of a chain starting at any point. The two-step minorization $P_{L,s}^2(u,\cdot)\ge\delta\mu_L$ makes its action on differences of probabilities a strict contraction in total variation, unless $\delta=1$, when it is already constant. Hence the stationary probability is unique. Applying the continuous two-step kernel to this probability gives a continuous density, bounded below by $\delta$. \end{proof} Reversibility means detailed balance with respect to the stationary probability, rather than merely the existence of that probability. \begin{theorem}[Reciprocity characterizes ellipsoids]\label{str:reversibility} For $L$ as above, the following conditions are equivalent. \begin{enumerate} \item $L$ is a centered ellipsoid. \item For some $s>0$, $P_{L,s}$ is reversible with respect to a probability measure. \item For every $s>0$, $P_{L,s}$ is self-adjoint on $L^2(\mu_L)$. \item For every $u,v,w\in\Sn$, the boundary incidence factors satisfy \begin{align} |\ip u{x_L(v)}|\,|\ip v{x_L(w)}|\,|\ip w{x_L(u)}| =|\ip v{x_L(u)}|\,|\ip w{x_L(v)}|\,|\ip u{x_L(w)}|. \label{str:cycles} \end{align} \end{enumerate} In the reversible case, the stationary probability is $\mu_L$. These characterizations are invariant under $GL(n,\R)$. \end{theorem} The elementary rigidity mechanism is local linear algebra, not a classification of compact transformation groups. \begin{lemma}[Local reciprocity]\label{str:localreciprocity} Suppose a continuous positive function $b$ on a connected open spherical patch $\Omega$ satisfies \[ b(u)\ip u{x_L(v)}=b(v)\ip v{x_L(u)}\qquad(u,v\in\Omega). \] Then $x_L(u)=b(u)A u$ on $\Omega$, for a symmetric matrix $A$. Locally, $h_L(u)^2$ is the restriction of a quadratic form. \end{lemma} \begin{proof} Set $y(u)=x_L(u)/b(u)$. Choose linearly independent $u_1,\ldots,u_n\in\Omega$, and let $U,Y$ be the matrices with columns $u_i,y(u_i)$, respectively. The reciprocity equations say that $U^{\mathsf T}Y$ is symmetric. Thus $A=YU^{-1}$ is symmetric. For every $v\in\Omega$ the same equations give $U^{\mathsf T}y(v)=Y^{\mathsf T}v=U^{\mathsf T}Av$, proving $y(v)=Av$. Since $h_L(u)=b(u)u^{\mathsf T}Au>0$ on the patch, \[ \nabla_{\Sn}\log h_L(u) =\frac{Au}{u^{\mathsf T}Au}-u =\nabla_{\Sn}\left(\tfrac12\log(u^{\mathsf T}Au)\right). \] Hence $h_L^2$ is a positive constant times $u^{\mathsf T}Au$ on each connected patch under consideration. \end{proof} \begin{proof}[Proof of Theorem~\ref{str:reversibility}] If $h_L(u)=\sqrt{u^{\mathsf T}Hu}$ with $H\succ0$, then $x_L(u)=Hu/h_L(u)$. Write \[ d_{n,s}=\int_{\Sn}|\ip uv|^s\dd\sigma(v). \] The cone measure of the ellipsoid is the image of spherical probability under $\theta\mapsto H^{1/2}\theta$ followed by the normal map. It follows that $m_{L,s}(u)=d_{n,s}h_L(u)^s$, and therefore \begin{equation}\label{str:ellipsoidkernel} p_{L,s}(u,v)= \frac{|u^{\mathsf T}Hv|^s}{d_{n,s}h_L(u)^s h_L(v)^s}. \end{equation} This is symmetric, proving the third condition. That condition implies the second. Suppose the second holds. Detailed balance implies stationarity; Lemma~\ref{str:stationary} gives a continuous positive density $w$ relative to $\mu_L$. Detailed balance, initially almost everywhere, holds everywhere by continuity and full support. Taking positive $s$th roots gives \[ b(u)|\ip u{x_L(v)}|=b(v)|\ip v{x_L(u)}|, \qquad b(u)=\left(\frac{w(u)}{m_{L,s}(u)}\right)^{1/s}>0. \] Around every point there is a connected patch on which both incidence factors are positive for every pair of points. Remove the absolute values there and apply Lemma~\ref{str:localreciprocity}. It shows that $h_L^2$ is locally a quadratic form. The forms agree on overlapping patches, since a quadratic polynomial vanishing on an open subset of the sphere vanishes identically. The sphere is connected for $n\ge2$, so there is a single symmetric $H$ with $h_L(u)^2=u^{\mathsf T}Hu$ everywhere. Positivity of $h_L$ makes $H$ positive definite. Thus the first condition holds. Symmetric kernels satisfy the three-cycle identity, and their row normalizations cancel from it. Taking $s$th roots proves the fourth condition from the third. Conversely, suppose \eqref{str:cycles}. Choose a small connected patch $\Omega$ with all incidence factors positive, fix $u_0\in\Omega$, and put \[ b(u)=\frac{\ip{u_0}{x_L(u)}}{\ip u{x_L(u_0)}}. \] The cycle identity gives the hypothesis of Lemma~\ref{str:localreciprocity} on $\Omega$. Its quadratic forms patch together as before, so $L$ is an ellipsoid. Uniqueness in Lemma~\ref{str:stationary} identifies the stationary probability in that case as $\mu_L$. For affine invariance, let $A\in GL(n,\R)$ and $T_Au=A^{-\mathsf T}u/|A^{-\mathsf T}u|$. Cone measure pushes forward under $T_A$, while $x_{AL}(T_Au)=Ax_L(u)$. Both the numerator and denominator in \eqref{str:chain} acquire the same factor $|A^{-\mathsf T}u|^{-s}$. Thus the chains are conjugate, proving the claimed invariance. \end{proof} For example, this gives a nonnegative affine invariant which vanishes exactly on centered ellipsoids. With $j_s(u,v)=w_{L,s}(u)p_{L,s}(u,v)$, set \begin{equation}\label{str:irreversibility} \mathfrak I_s(L)=\frac12\iint \bigl(\sqrt{j_s(u,v)}-\sqrt{j_s(v,u)}\bigr)^2 \mu_L(\dd u)\mu_L(\dd v). \end{equation} The two edge densities have total mass one, so $0\le\mathfrak I_s(L)\le1$. Theorem~\ref{str:reversibility} shows that $\mathfrak I_s(L)=0$ if and only if $L$ is a centered ellipsoid. The unique stationary law in this construction exists for every regular $L$; its existence alone does not imply reversibility. \subsection{A sharp quadratic identity} There is a second, entirely explicit form of the same geometric rigidity. Here suppose $L=-L$, and use spherical probability $\sigma$. Let $P_\ell$ denote projection onto degree-$\ell$ spherical harmonics. Put \begin{align} F(u)&=\tfrac12h_L(u)^2,& Y(u)&=\nabla F(u)=h_L(u)x_L(u),\notag\\ H_L&=\int_{\Sn}D^2F(u)\dd\sigma(u),& g_L(u)&=h_L(u)^2-u^{\mathsf T}H_Lu,\label{str:quadraticdata}\\ \mathfrak R(L)&=\iint \bigl(\ip u{Y(v)}-\ip v{Y(u)}\bigr)^2 \dd\sigma(u)\dd\sigma(v).\notag \end{align} Derivatives of homogeneous functions in this subsection are ambient derivatives unless a spherical subscript is present. \begin{theorem}[Exact reciprocity identity]\label{str:quadraticidentity} The matrix $H_L$ is positive definite, and $u^{\mathsf T}H_Lu=(P_0+P_2)h_L^2$ is the orthogonal projection of $h_L^2$ onto the restrictions of quadratic forms. Hence $E_L$ below is the unique best ellipsoid for this squared-support $L^2$ approximation. Moreover, \begin{align} \mathfrak R(L) &=\frac2n\int|Y(u)-H_Lu|^2\dd\sigma(u)\notag\\ &=\frac1{2n}\int\bigl(|\nabla_{\Sn}g_L|^2+4g_L^2\bigr)\dd\sigma \label{str:exactidentity}\\ &=\frac1{2n}\sum_{\substack{\ell\ge4\\\ell\ { m even}}} \bigl(\ell(\ell+n-2)+4\bigr)\|P_\ell h_L^2\|_2^2.\notag \end{align} Consequently \begin{equation}\label{str:sharpstability} \|h_L^2-h_{E_L}^2\|_2^2 \le\frac{n}{2(n+3)}\mathfrak R(L),\qquad h_{E_L}(u)=\sqrt{u^{\mathsf T}H_Lu}. \end{equation} The constant is sharp in every dimension $n\ge2$. In particular, $\mathfrak R(L)=0$ if and only if $L$ is a centered ellipsoid. \end{theorem} \begin{proof} Since $h_L>0$ and its tangential Hessian is positive, \[ D^2F=\nabla h_L\nabla h_L^{\mathsf T}+h_LD^2h_L\succ0. \] This proves $H_L\succ0$. Homogeneity and the divergence theorem on the Euclidean unit ball give \begin{equation}\label{str:matrixmoment} H_L=n\int Y(u)u^{\mathsf T}\dd\sigma(u). \end{equation} Indeed the Hessian is homogeneous of degree zero, so its ball average equals its spherical average. One may apply divergence on annuli and let the inner radius tend to zero, avoiding differentiability at the origin. In particular the matrix on the right is symmetric. For any square-integrable vector field $Y$, expansion of the double integral in \eqref{str:quadraticdata} gives \[ \mathfrak R(L)=\frac2n\int|Y|^2\dd\sigma -2\tr\left(\left(\int Yu^{\mathsf T}\dd\sigma\right)^2\right). \] Using \eqref{str:matrixmoment} yields the first equality in \eqref{str:exactidentity}; it is also the least-squares identity for approximation of $Y$ by a linear vector field. For completeness write $f=h_L^2$, $\bar f=\int f\dd\sigma$, and $M_f=\int f(u)uu^{\mathsf T}\dd\sigma(u)$. Spherical integration by parts gives $\int u_i(\nabla_{\Sn}f)_j\dd\sigma=n(M_f)_{ij}-\delta_{ij}\bar f$. Since $Y=fu+\nabla_{\Sn}f/2$, \eqref{str:matrixmoment} becomes \begin{equation}\label{str:projectionmatrix} H_L=\frac{n(n+2)}2M_f-\frac n2\bar f\Id. \end{equation} The spherical fourth-moment formula identifies $u^{\mathsf T}H_Lu=(P_0+P_2)f$. Thus $g_L$ has no components of degree zero or two. Also \[ Y-H_Lu=g_Lu+\tfrac12\nabla_{\Sn}g_L, \] whose two terms are pointwise orthogonal. This gives the second equality in \eqref{str:exactidentity}. The eigenvalues of the spherical Laplacian give the last one. Evenness excludes odd degrees. The first remaining eigenvalue is $4(n+2)$, and hence \[ \mathfrak R(L)\ge\frac{2(n+3)}n\|g_L\|_2^2, \] which is \eqref{str:sharpstability}. For sharpness take $h_L(u)=\sqrt{1+\epsilon Z_4(u)}$, where $Z_4$ is a nonzero degree-four spherical harmonic and $\epsilon\ne0$ is sufficiently small. This is the support function of a regular symmetric convex body, by $C^2$ closeness to the ball. Its defect $g_L=\epsilon Z_4$ attains equality. \end{proof} Thus squared support functions turn the ellipsoid family into the positive cone in the linear space of quadratic forms. The exact identity is global, rather than a linearization at the ball; its constant has no exceptional dimensions. The spherical defect itself depends on the Euclidean coordinates. An affine invariant version is obtained by applying it to $\widehat L=\Sigma_L^{-1/2}L$, where $\Sigma_L=\Cov(U_L)$. Indeed $\widehat{AL}=O\widehat L$ for an orthogonal $O$. The ellipsoid assignment $L\mapsto\Sigma_L^{1/2}E_{\widehat L}$ is therefore affine equivariant and returns $L$ whenever $L$ is an ellipsoid. \section{Affine covariance as a spectral principle}\label{sec:affinestructure} The eigenvalue and orthogonality used below are consequences of affine covariance and homogeneity. They hold for all centroid moments. For $s\ge1$ define the volume-normalized $L_s$ centroid body by \[ h_{\Gamma_s L}(u)^s=\E|\ip u{U_L}|^s. \] Suppose a regular $L$ satisfies $\Gamma_s L=cL$, and set $F_A(u)=\ip u{Ax_L(u)}/h_L(u)$. \begin{theorem}[Affine and moment identities]\label{str:affineidentity} For every real matrix $A$, \begin{equation}\label{str:affineeigen} P_{L,s}F_A=\frac{sF_A+\tr A}{n+s},\qquad \int F_A\dd\mu_L=\frac{\tr A}{n}. \end{equation} The kernel of $A\mapsto F_A$ is the Lie algebra of $\Aut(L)$. For every continuously differentiable polynomial $T$, \begin{equation}\label{str:momentidentity} \int F_A(u)T(x_L(u))\mu_L(\dd u) =\frac1n\E\bigl[(\tr A)T(U_L)+DT(U_L)[AU_L]\bigr]. \end{equation} In inertia position, the rotational functions $F_A$, $A^{\mathsf T}=-A$, are orthogonal to constants and all boundary quadratic functions, and span an invariant subspace of dimension $n(n-1)/2-\dim\Aut(L)$ on which $P_{L,s}$ acts by $s/(n+s)$. \end{theorem} \begin{proof} The divergence theorem applied to $Ax\,|\ip ux|^s$ gives \[ \int_{\partial L}|\ip ux|^s\ip{Ax}{\nu(x)}\dd S(x) =(\tr A)c^s|L|h_L(u)^s +s c^s|L|h_L(u)^{s-1}\ip u{Ax_L(u)}. \] Here differentiation of the fixed-point equation was used for the second term; for $s=1$ differentiation is justified by dominated convergence. Divide by $n|L|m_{L,s}(u)$ and use \eqref{str:chainnormalization}. This proves the first identity in \eqref{str:affineeigen}. Applying divergence to $Ax$, or to $Ax\,T(x)$, proves the second and \eqref{str:momentidentity}. Finally $F_A=0$ says that the derivative of $h_L$ along $e^{tA^{\mathsf T}}u$ vanishes, equivalently $e^{tA}L=L$. In inertia position these automorphisms are orthogonal. Taking $T(x)=xx^{\mathsf T}$ in \eqref{str:momentidentity} gives \[ \int F_Axx^{\mathsf T}\dd\mu_L =\frac1n\bigl((\tr A)\Sigma_L+A\Sigma_L+\Sigma_LA^{\mathsf T}\bigr), \] which vanishes for skew $A$ and scalar $\Sigma_L$. Rank--nullity proves the dimension assertion. \end{proof} \begin{corollary}[A spectral certificate for symmetry]\label{str:spectralcertificate} Let $\Pi$ be orthogonal projection in $L^2(\mu_L)$ onto constants and boundary quadratic functions. Put $B_{L,s}=P_{L,s}(I-\Pi)$ and $\lambda_s=s/(n+s)$. In inertia position, \begin{equation}\label{str:HSbound} \left(\frac{n(n-1)}2-\dim\Aut(L)\right)\lambda_s^2 \le\|B_{L,s}\|_{\mathrm{HS}}^2. \end{equation} If $\|B_{L,s}\|_{L^2\to L^2}<\lambda_s$, then $L$ is a ball in this position, and hence an ellipsoid before normalization. \end{corollary} \begin{proof} For an orthonormal basis $e_j$ of the rotational subspace, $\Pi e_j=0$ and $B_{L,s}e_j=\lambda_s e_j$. The Hilbert--Schmidt norm bounds the sum of the squared norms of these images, proving \eqref{str:HSbound}. The strict operator-norm bound forces every rotational function to vanish. Thus every one-parameter rotation preserves $L$, and $SO(n)$ invariance makes $L$ a ball. This argument uses neither reversibility nor stationarity of the reference cone measure. \end{proof} \subsection{Relation to the fixed-point classification} For the ordinary centroid equation, Theorem~\ref{str:affineidentity} explains the universal eigenvalue $1/(n+1)$ and the role of quadratic regression. Corollary~\ref{str:spectralcertificate} is the abstract form of the symmetry estimates in the classification proof. Theorem~\ref{str:reversibility} and Theorem~\ref{str:quadraticidentity} identify their geometric target: a reciprocal boundary map, equivalently a quadratic squared support function. A shorter proof of the fixed-point theorem would follow from a direct implication \begin{equation}\label{str:directtarget} \Gamma L=cL\quad\Longrightarrow\quad P_{L,1}\ \hbox{is reversible}, \qquad\hbox{or directly}\quad\mathfrak R(L)=0. \end{equation} No direct proof of this implication is supplied here. The detailed classification argument below is still needed; after that argument, \eqref{str:directtarget} follows as a corollary. Thus the reciprocity theorems are independent structural characterizations, and are not being used as an unproved replacement for the difficult step. There is a precise warning against confusing an affine identity with detailed balance. At a fixed body, any stationary probability $\pi$ for $P_{L,s}$ satisfies, by \eqref{str:affineeigen}, \[ \int F_A\dd\pi=\frac{\tr A}{n},\qquad \int\frac{x_L(u)u^{\mathsf T}}{h_L(u)}\pi(\dd u)=\frac1n\Id. \] Cone measure satisfies the same moment identities. Equality of these finitely many moments is not by itself an identification of the two measures or a proof of detailed balance. \section{A signed spherical moment gap and low dimensions}\label{sec:finite} \begin{proposition}\label{prop:lowdim} If $2\le n\le25$ and $K$ satisfies \eqref{eq:fixed}, then $K$ is a centered ellipsoid and $c=a_n$. \end{proposition} Let $\sigma$ denote spherical probability measure and define \begin{equation}\label{pre:cosine} b_n=\int_{\Sn}|\ip uv|\dd\sigma(v) =\frac{2\kappa_{n-1}}{n\kappa_n},\qquad \C f(u)=b_n^{-1}\int_{\Sn}|\ip uv|f(v)\dd\sigma(v). \end{equation} Thus $\C1=1$ and $a_n=nb_n/(n+1)$. For $r=\rho_K$, polar integration gives \begin{equation}\label{pre:radialidentity} h_{\T K}=\frac{\C(r^{n+1})}{\int r^n\dd\sigma}. \end{equation} Inertia position implies the exact identity \begin{equation}\label{pre:quadraticcancel} P_2(r^{n+2})=0, \end{equation} where $P_\ell$ denotes orthogonal projection onto degree-$\ell$ spherical harmonics: integrate any homogeneous harmonic quadratic over $K$ in polar coordinates to obtain \eqref{pre:quadraticcancel}. \begin{lemma}\label{pre:multipliers} The even cosine-transform multipliers are \begin{equation}\label{pre:multiplierformula} \mu_0=1,\qquad \mu_{2j}=(-1)^{j-1} \frac{\Gamma(j-1/2)\Gamma((n+1)/2)} {2\sqrt\pi\,\Gamma(j+(n+1)/2)}\quad(j\ge1). \end{equation} In particular, \[ \mu_2=\frac1{n+1},\quad \mu_4=-\frac1{(n+1)(n+3)},\quad \mu_6=\frac3{(n+1)(n+3)(n+5)}, \quad \frac{\mu_{\ell+2}}{\mu_\ell}=-\frac{\ell-1}{\ell+n+1} \] for even $\ell\ge2$. Thus $\mu_\ell\le\mu_6$ for every even $\ell\ge4$. \end{lemma} \begin{proof} For $n\ge3$, formula~\eqref{pre:multiplierformula} follows from Funk--Hecke; see also \cite[Section~3]{Reuter} with normalization \eqref{pre:cosine}. For $n=2$, the Fourier series of $|\cos t|$ gives $\mu_{2j}=(-1)^{j-1}/(4j^2-1)$, which is the same formula. The recurrence follows by the Gamma identity. Its ratio has absolute value less than one, and the signs alternate after degree two. \end{proof} In this section $K$ is a fixed body in inertia position. Write $r=\rho_K$ and \begin{equation}\label{low:moments} A_j=\int_{\Sn}r^{n+j}\dd\sigma\quad(j=0,1,2),\qquad f=r^{n+1},\qquad \Delta=A_0A_2-A_1^2. \end{equation} Cauchy--Schwarz gives $\Delta\ge0$, with equality exactly when $r$ is constant. \begin{lemma}\label{low:P2} Under \eqref{pre:quadraticcancel}, \begin{equation}\label{low:P2bound} \norm{P_2 f}_2^2\le\frac{n+2}{2}\Delta. \end{equation} \end{lemma} \begin{proof} Put $\dd\nu=r^{n+2}\dd\sigma/A_2$ and $g=1/r$. Then $\E_\nu vv^{\mathsf T}=\Id/n$ and $\Var_\nu g=\Delta/A_2^2$. The trace-free symmetric matrix \[ S=\E_\nu[(g-\E_\nu g)vv^{\mathsf T}] \] satisfies, for every trace-free symmetric $U$, \[ |\tr(US)|^2\le\Var_\nu(g)\E_\nu(v^{\mathsf T}Uv)^2 \le\frac{\Var_\nu(g)}n\tr(U^2). \] The second inequality uses $(v^{\mathsf T}Uv)^2\le v^{\mathsf T}U^2v$. Taking $U=S$ gives $\tr(S^2)\le\Delta/(nA_2^2)$. The trace-free moment matrix of $f$ is $M_f=\int f(v)(vv^{\mathsf T}-\Id/n)\dd\sigma=A_2S$. The spherical fourth-moment identity yields \[ P_2f(u)=\frac{n(n+2)}2u^{\mathsf T}M_fu, \qquad \norm{P_2f}_2^2=\frac{n(n+2)}2\tr(M_f^2). \] Substitution proves \eqref{low:P2bound}. \end{proof} \begin{lemma}\label{low:variance} If $\max r/\min r\le q$, then \begin{equation}\label{low:variancebound} \Var_\sigma(f)\le\Lambda_n(q)\Delta, \qquad \Lambda_n(q)=q^{-n}\left(\sum_{j=0}^nq^j\right)^2. \end{equation} Here $\Lambda_n(1)=(n+1)^2$. \end{lemma} \begin{proof} For positive $s,t$ with $s/t\in[q^{-1},q]$, \[ \frac{(s^{n+1}-t^{n+1})^2}{s^nt^n(s-t)^2} =\left(\sum_{j=0}^n(s/t)^{j-n/2}\right)^2\le\Lambda_n(q). \] The expression is invariant under $s/t\mapsto t/s$ and is increasing for $s/t\ge1$: opposite powers pair into increasing hyperbolic cosines. Integrate the undivided inequality and use \[ \Var_\sigma f=\frac12\iint(f(u)-f(v))^2\dd\sigma(u)\dd\sigma(v), \quad \Delta=\frac12\iint r(u)^nr(v)^n(r(u)-r(v))^2 \dd\sigma(u)\dd\sigma(v). \] \end{proof} \begin{proposition}\label{low:criterion} A fixed body is an ellipsoid if its inertia-position radial ratio is at most $q$ and \begin{equation}\label{low:criterionformula} 6\Lambda_n(q)
0$ and, for real $x\ge3$, put
\[
F(x)=\log\frac{6\sinh^2((x+1)t)}{p(x)\sinh^2t}.
\]
For integer $n$, $e^{F(n)}=6\Lambda_n(q_*)/p(n)$.
Using $\sinh y\ge y$ and differentiating twice gives
\[
F''(x)\ge\frac{W(x)}{(x+1)^2p(x)^2},\qquad
W(x)=x^6+6x^5-5x^4-60x^3+20x^2+276x+156.
\]
Indeed, the numerator is
$(x+1)^2(p'(x)^2-p''(x)p(x))-2p(x)^2$.
The polynomial $x^3+6x^2-5x-60$ is increasing and equals $6$ at $x=3$.
Writing $W=x^3(x^3+6x^2-5x-60)+20x^2+276x+156$ proves $F''>0$.
Hence the maximum of $F$ on $[3,25]$ is at an endpoint.
At $n=3$, monotonicity in $q$ gives
\[
6\Lambda_3(q_*)<6\Lambda_3(5/4)
=6\cdot\frac{136161}{8000}<159=p(3).
\]
At $n=25$, the integer inequality $601^{13}<11\cdot500^{13}$ gives
\[
\Lambda_{25}(q_*)
=\frac{q_*}{(q_*-1)^2}(q_*^{13}-q_*^{-13})^2
<\frac{300500}{10201}\left(\frac{120}{11}\right)^2.
\]
The desired comparison with $p(25)=21081$ is precisely
$25963200000<26020721001$.
Both endpoint values are negative, so $F<0$ on the whole interval.
\end{proof}
\begin{proof}[Proof of Proposition~\ref{prop:lowdim}]
Put $K$ in inertia position.
For $n=2$, Lemma~\ref{pre:moments} gives
$Q_2=\sqrt{9/8}<5/4$, and the exact comparison
\[
6\Lambda_2(5/4)=\frac{11163}{200}<82=p(2)
\]
allows us to apply Proposition~\ref{low:criterion}.
Now suppose $3\le n\le25$. Lemma~\ref{pre:moments} yields
\[
(\max r/\min r)^2\le Q_n^2\le Q_{25}^2=13/9<(601/500)^2;
\]
the last comparison is $3250000<3250809$.
Proposition~\ref{low:criterion} and Lemma~\ref{low:endpoints} show that
$K$ is a ball in this position. Undoing the linear map gives an ellipsoid;
\eqref{eq:equivariance} then gives $c=a_n$.
\end{proof}
\section{The boundary operator and quadratic orthogonality}\label{sec:boundary}
Work in inertia position \eqref{eq:inertia}.
Write $h=h_K$ and $x(u)=\nabla h(u)$, with $h$ extended
one-homogeneously to $\R^n\setminus\{0\}$.
The regularity needed here follows directly from slicing. For unit
$u$ and $v\perp u$,
\begin{equation}\label{eq:slice}
D^2h_{\Gamma K}(u)[v,v]
=\frac2V\int_{K\cap u^\perp}\ip vx^2\dd\mathcal H^{n-1}(x)>0
\quad(v\ne0).
\end{equation}
The section integral is continuous in $u,v$: polar integration in the
section expresses it as an integral of the continuous radial function
of $K$ to the power $n+1$. Thus $h_{\Gamma K}$ is $C^2$ away from
zero with positive tangential Hessian. By \eqref{eq:fixed}, the same
is true for $h$. In particular $x(u)$ parametrizes the boundary by its
outer normal, and its cone probability measure is
\begin{equation}\label{eq:cone}
\mu(\dd u)=\frac{h(u)}{nV}S_K(\dd u).
\end{equation}
This measure has a continuous positive density and full support.
For a real matrix $A$, define
\begin{equation}\label{eq:affine}
F_A(u)=\frac{\ip u{Ax(u)}}{h(u)}.
\end{equation}
Let $Q$ have kernel, relative to $\mu$,
\begin{equation}\label{eq:kernel}
q(u,v)=\frac{n}{(n+1)c}\frac{|\ip u{x(v)}|}{h(u)}.
\end{equation}
It is a compact integral operator on $L^2(\mu)$.
\begin{lemma}[Affine regression]\label{lem:regression}
One has $Q1=1$ and, for every real matrix $A$,
\begin{equation}\label{eq:regression}
QF_A=\frac{F_A+\tr A}{n+1},\qquad
\int F_A\dd\mu=\frac{\tr A}{n}.
\end{equation}
The kernel of $A\mapsto F_A$ is the Lie algebra $\mathfrak g_K$ of
$\Aut(K)$. In inertia position $\mathfrak g_K\subset\mathfrak{so}(n)$.
\end{lemma}
\begin{proof}
This is the case $s=1$ of Theorem~\ref{str:affineidentity}, since
\eqref{str:chainnormalization} identifies $Q=P_{K,1}$.
The regularity needed there was established in \eqref{eq:slice}.
\end{proof}
\begin{lemma}[Quadratic orthogonality]\label{lem:orthogonal}
For every skew-symmetric matrix $A$,
\begin{equation}\label{eq:orthogonal}
\int F_A\dd\mu=0,\qquad
\int F_A(u)x(u)x(u)^{\mathsf T}\mu(\dd u)=0.
\end{equation}
Consequently the invariant subspace
\[
\mathcal R=\{F_A:A\in\mathfrak{so}(n)\},\qquad
Q|_{\mathcal R}=\frac1{n+1}\Id,
\]
is orthogonal to constants and to all functions $u\mapsto x(u)^{\mathsf T}Bx(u)$.
Its dimension is
\begin{equation}\label{eq:rotationdimension}
m:=\dim\mathcal R=\frac{n(n-1)}2-d.
\end{equation}
\end{lemma}
\begin{proof}
The moment identity \eqref{str:momentidentity}, with $T(x)=xx^{\mathsf T}$, gives, for $\Sigma=\Cov(U)$,
\begin{align*}
\int F_A(u)x(u)x(u)^{\mathsf T}\mu(\dd u)
&=\frac1{nV}\int_{\partial K}xx^{\mathsf T}\ip{Ax}{\nu(x)}\dd S(x)\\
&=\frac1n\bigl((\tr A)\Sigma+A\Sigma+\Sigma A^{\mathsf T}\bigr).
\end{align*}
For skew $A$ this vanishes by \eqref{eq:inertia}. The other assertions
follow from Lemma~\ref{lem:regression} and rank--nullity.
\end{proof}
\begin{theorem}[Quadratic symmetry bound]\label{thm:dimension}
For a fixed body in dimension $n\ge26$,
\begin{equation}\label{eq:dimension}
d>D(n):=\frac{n(n-1)}2-\frac6{25}(n+1)^2
=\frac{13n^2-49n-12}{50}.
\end{equation}
\end{theorem}
\section{A scalar quadratic approximation}
\begin{lemma}[Exponential comparison]\label{lem:exponential}
Let $Y\ge0$ have a log-concave density and $\E Y=1$, and let
$\xi$ have the exponential density $e^{-y}$ on $[0,\infty)$.
For every convex function $H$ for which the expectations exist,
\begin{equation}\label{eq:convexorder}
\E H(Y)\le\E H(\xi).
\end{equation}
\end{lemma}
\begin{proof}
Write $S(t)=\mathbb P(Y>t)$. Log-concavity of the density implies
that $S$ is log-concave. For example,
$S(t)/f(t)=\int_0^\infty f(t+s)/f(t)\dd s$ is nonincreasing on
the positive support, so the hazard rate is nondecreasing.
Since $S(0)=1$, the concave function $\log S(t)+t$ shows that
$S(t)-e^{-t}$ changes sign at most once, from positive to negative.
Its integral is zero because $\E Y=\E\xi=1$.
It follows that
\[
\E(Y-a)_+=\int_a^\infty S(t)\dd t\le e^{-a}
=\E(\xi-a)_+\qquad(a\ge0).
\]
Together with equality of means, this proves \eqref{eq:convexorder}
by the representation of a convex function as an affine function plus
a positive integral of hinges. Approximation gives the asserted
integrable generality.
\end{proof}
Put
\begin{equation}\label{eq:polynomials}
R(y)=y-\frac23-\frac{y^2}{5},\qquad
P(y)=R(y)^2,\qquad P_t(y)=P(y)+tyP'(y).
\end{equation}
\begin{lemma}[Uniform scalar bound]\label{lem:scalar}
For $Y$ as in Lemma~\ref{lem:exponential} and $0\le t\le1/26$,
\begin{equation}\label{eq:scalar}
\E P_t(Y)<\frac6{25}(1+t)^2.
\end{equation}
\end{lemma}
\begin{proof}
Set $z=11/6$. For $\eta\in\{0,1/26\}$ let $L_\eta$ be the tangent
line to $P_\eta$ at $z$, and put $H_\eta=\max(P_\eta,L_\eta)$.
Direct factorization gives
\begin{align}
P_0(y)-L_0(y)
&=\frac{(y-z)^2}{300}(12y^2-76y+61),\label{eq:factor0}\\
P_{1/26}(y)-L_{1/26}(y)
&=\frac{(y-z)^2}{780}(36y^2-216y+151).\label{eq:factor26}
\end{align}
In each case the quadratic factor has two roots $r_- n/2,\qquad k:=\dim H_*=n-p\ge2,\qquad
G=O(W)\times G_*,
\end{equation}
where $G=\Aut(K)$, $G_*\subset O(H_*)$ contains $-\Id_{H_*}$ and
contains no hyperplane reflection. In particular $W$ is $G$-invariant.
There are an origin-symmetric convex body $D\subset H_*$ and an even
concave function $r:D\to[0,\infty)$, positive on its interior, such that
\begin{equation}\label{eq:profile}
K=\{(y,z)\in W\oplus H_*:z\in D,\ |y|\le r(z)\}.
\end{equation}
The function $r$ is continuous on $D$ and vanishes on $\partial D$.
\end{theorem}
\begin{proof}
Proposition~\ref{prop:largeblock} supplies an independent rotation
subspace $E$ of dimension greater than $n/2$.
We show that any additional reflection normal $v\notin E$ enlarges it.
Choose a unit vector $e\in E\cap v^\perp$; this is possible since
$\dim E\ge2$. The reflections with normals $e$ and $v$ preserve $K$.
Lemma~\ref{lem:tworeflections} gives the plane rotation generator
$e\wedge v$. Subtracting the generator $e\wedge P_Ev$ already in
$\mathfrak{so}(E)$ gives $e\wedge P_{E^\perp}v$.
Brackets with $\mathfrak{so}(E)$ generate
$\mathfrak{so}(E\oplus\R P_{E^\perp}v)$.
The existing reflection with normal $e$ then supplies the full
independent orthogonal group of this enlarged subspace.
Iterating over a finite spanning set of reflection normals proves
$O(W)\times\{\Id\}\subset G$.
Conjugation carries a preserving reflection to a preserving reflection,
so $G$ preserves $W$ and $H_*$. Cancelling the $O(W)$ component of each
$g\in G$ proves the direct-product assertion. Central symmetry gives
$-\Id_{H_*}\in G_*$. A reflection in $G_*$ would have a normal both in
$H_*$ and in $W$, which is impossible. If $k=1$, then
$-\Id_{H_*}$ is just such a reflection. If $k=0$, invariance under
$O(n)$ makes $K$ a ball. Thus $k\ge2$.
Independent $O(W)$ invariance makes every fiber a centered ball.
Convexity of $K$ gives concavity of its radius $r$, and central
symmetry gives evenness. Interior continuity follows from concavity.
At a boundary point of $D$ the fiber lies in a supporting face of $K$;
strict convexity of $K$ forces its radius to vanish. Compactness of $K$
then gives continuity at those boundary points as well.
\end{proof}
\begin{corollary}\label{cor:irreducible}
For $n\ge26$, if the full automorphism group of a fixed body is
irreducible, the body is an ellipsoid.
\end{corollary}
\begin{proof}
In inertia position, Theorem~\ref{thm:canonical} would otherwise
give a proper, nonzero invariant subspace $W$.
\end{proof}
\section{The complementary action and the two-thirds bound}
We say that a compact connected group $H\subset SO(k)$ has an
\emph{independent sphere-transitive subspace} if there is an orthogonal
decomposition $\R^k=E\oplus E^\perp$, with $\dim E\ge2$, and a
subgroup of $H$ fixing $E^\perp$ pointwise and transitive on the
unit sphere of $E$.
\begin{lemma}\label{lem:noblock}
Suppose $H\subset SO(k)$ is closed and connected and has no independent
sphere-transitive subspace.
If $k\ge10$, then $\dim H\le g(k)$.
If $k=9$, then $\dim H\le9$.
\end{lemma}
\begin{proof}
First suppose $k\ge10$ and, for a contradiction, $d_H:=\dim H>g(k)$.
Decompose its real representation into irreducible summands of
dimensions $p_i$, and put $p=\max p_i$.
Faithfulness gives $d_H\le\sum_i p_i(p_i-1)/2$.
If every $p_i\le k/2$, the elementary partition estimate used in
Proposition~\ref{prop:largeblock} leaves only $k=2m$ and two
$m$-dimensional summands. This estimate holds already for $m\ge5$:
for odd $k=2m+1$ the maximum is $m(m-1) g(p)+\frac{q(2p-q-1)}4.
\end{equation}
If $p\ge10$, Lemma~\ref{lem:groupgap} gives $SO(p)$ or a group
containing $SU(p/2)$. Lift the corresponding simple ideal to
$\mathfrak h$. In the orthogonal case its action on the $q$-dimensional
complement is zero by the dimension comparison with $\mathfrak{so}(q)$.
In the unitary case it is zero by Lemma~\ref{lem:smallrep}.
This gives an independent sphere-transitive action, a contradiction.
The remaining possibilities have $6\le p\le9$.
For $p=6$, \eqref{eq:projectedgap} and Lemma~\ref{lem:smallgroups}
give $SO(6)$ or a group containing $SU(3)$; the corresponding simple
factor has no nontrivial representation on a complement of dimension
$q<6$. For $p=7$, the alternatives are $SO(7)$ and $G_2$, and the
same argument applies since their smallest nontrivial real
representations have dimension seven.
For $p=9$, Lemma~\ref{lem:smallgroups} forces $L=SO(9)$.
For $p=8$, we have $q\ge2$ because $k\ge10$.
If $q=2$ or $3$, \eqref{eq:projectedgap} gives
$\dim L>16$ or $\dim L>19$, respectively; hence
$L=Spin(7)$ or $SO(8)$.
Their relevant simple ideals act trivially on the complement.
If $q\ge4$, the same bound gives $\dim L>21$, so $L=SO(8)$.
Every case again gives the forbidden independent action.
This proves the assertion for $k\ge10$.
Now let $k=9$ and suppose $d_H\ge10$.
If the action is irreducible, Lemma~\ref{lem:smallgroups} gives $SO(9)$.
Otherwise let $p$ be the largest irreducible dimension.
For $p=8$, the complement is one dimensional, and the image has
dimension at least ten; every group in the corresponding row of Lemma~\ref{lem:smallgroups}
is sphere-transitive, acting independently of that complement.
For $p=7$, the image has dimension at least nine, and its $G_2$ or
$SO(7)$ simple factor acts trivially on the two-dimensional complement.
For $p=6$, the image has dimension at least seven, and its $SU(3)$
or $SO(6)$ simple factor acts trivially on the three-dimensional
complement. For $p=5$, the image has dimension at least four, and
must be $SO(5)$; it cannot act nontrivially on a four-dimensional
complement. All these cases are impossible.
Finally suppose every irreducible summand has dimension at most four.
The only partitions whose ambient block algebra has dimension at
least ten are $4+4+1$ and $4+3+2$.
For $4+3+2$, dimension at least ten forces the full block algebra,
giving an independent action.
For $4+4+1$, if one projection to $\mathfrak{so}(4)$ is proper,
its dimension is at most four. Dimension at least ten therefore
forces a full product of a four-dimensional projection and the other
$\mathfrak{so}(4)$.
If both projections are onto, use
$\mathfrak{so}(4)=\mathfrak{su}(2)\oplus\mathfrak{su}(2)$.
Its quotients have dimensions $0,3,6$, so a subdirect product of two
copies has dimension $12,9$, or $6$.
Dimension at least ten forces dimension twelve and the full product.
Again an independent sphere-transitive action is present.
This proves $\dim H\le9$.
\end{proof}
\begin{proposition}\label{prop:twothirds}
For a nonball fixed body in inertia position with $n\ge26$, the
canonical rotation subspace in Theorem~\ref{thm:canonical} has
\begin{equation}\label{eq:twothirds}
p\ge\lceil2n/3\rceil,\qquad
p\ge19\quad\hbox{when }n=27.
\end{equation}
\end{proposition}
\begin{proof}
Set $H=G_*^0\subset SO(k)$. It has no independent sphere-transitive
subspace. Indeed, such a subgroup has exactly the same point orbits
as the independent orthogonal group on that subspace; invariance
of the profile body under it would give a hyperplane reflection in
$G_*$, contrary to Theorem~\ref{thm:canonical}.
If $k\le8$, then $p=n-k\ge n-8\ge2n/3$.
If $k\ge9$, Lemma~\ref{lem:noblock} gives
$\dim G_*\le g(k)$, including $k=9$ since $90$, direct integration in the first spherical coordinate gives
\[
\partial_B\psi_p(A,B)=\beta_p
\left(1-\frac{B^2}{A^2}\right)_+^{(p-1)/2},\qquad
\psi_p(A,0)=0.
\]
Indeed, the density of $\theta_1$ is
$c_p(1-t^2)^{(p-3)/2}$ on $(-1,1)$, where
$c_p=\Gamma(p/2)/(\sqrt\pi\,\Gamma((p-1)/2))$.
For $00$.
The cone measure is invariant under independent $O(W)$ rotations.
Moreover $x_W(v)$ is a positive multiple of $v_W$ whenever $v_W\ne0$:
equivariance gives parallelism, and strict convexity and reflection
symmetry give the sign. Thus the $W$ directions of the boundary point
and its normal coincide outside a null set.
Conditional on the rotation-invariant coordinates, this direction
is uniform. Consequently the first-harmonic projection is orthogonal
on $L^2(\mu)$ as well as for the interior law.
All other $W$ harmonics in a row of $Q$ are orthogonal to
$\mathcal R_\times$.
Let $e_1,\ldots,e_{pk}$ be an orthonormal basis of $\mathcal R_\times$.
Subtract the optimal boundary quadratic above from the first-harmonic
part of each row of $Q$. Bessel's inequality, the kernel normalization
\eqref{eq:kernel}, and \eqref{eq:crossregression} yield
\[
\frac{1}{(n+1)^2}\sum_j e_j(u)^2
\le \frac{n(n+2)p\beta_p^2\tau\Delta_{n,p,k}}
{(n+1)^2c^2}\frac{|u_{H_*}|^2}{h(u)^2}.
\]
Integrate in $u$ and use the exact identity
\[
\int\frac{|u_{H_*}|^2}{h(u)^2}\mu(\dd u)
=\frac1n\tr(P_{H_*}J_\Phi P_{H_*}).
\]
Then apply \eqref{eq:fisherupper}:
\begin{align*}
\frac{pk}{(n+1)^2}
&\le\frac{(n+2)p\beta_p^2\tau\Delta_{n,p,k}}
{(n+1)^2c^2}\tr(P_{H_*}J_\Phi P_{H_*})\\
&\le\frac{(n+2)p\beta_p^2 k\Delta_{n,p,k}}
{(n+1)^2\gamma}.
\end{align*}
Cancelling the positive factors proves \eqref{eq:criterion}.
No self-adjointness or invariant-probability assertion for $Q$ is used.
\end{proof}
\section{Excluding every proper rotation subspace}\label{sec:closing}
\begin{proposition}\label{prop:closing}
For every $n\ge26$ and every integer $p$ satisfying
\eqref{eq:twothirds}, with $k=n-p\ge2$,
\begin{equation}\label{eq:closing}
\Delta_{n,p,k}(n+2)\beta_p^2<\frac{87}{500}<\gamma.
\end{equation}
\end{proposition}
\begin{proof}
Both $\beta_p$ and
$\varepsilon^2=(n-p+3)/(p(n+4))$ decrease with $p$.
For $\beta_p$, couple the spherical vectors by normalizing the
same independent standard Gaussian coordinates: the absolute first
coordinate decreases when an extra coordinate is included in the
normalizing Euclidean norm.
First suppose $n\ge32$.
By $p\ge2n/3$,
\[
\varepsilon^2\le\frac{n+9}{2n(n+4)}
\le\frac{41}{2304},\qquad
\varepsilon<\frac{267}{2000},\qquad
\sqrt{\frac{1+\varepsilon^2}{14}}<\frac{27}{100}.
\]
The first rational function is decreasing for $n>0$.
Log-convexity of the Gamma function gives
$\Gamma(p/2)^2\le
\Gamma((p-1)/2)\Gamma((p+1)/2)$, hence
$\beta_p^2\le2/[\pi(p-1)]$.
Since $(n+2)/(2n/3-1)$ is decreasing,
\[
(n+2)\beta_p^2
\le\frac{2(n+2)}{\pi(2n/3-1)}
\le\frac{204}{61\pi}<\frac{16}{15};
\]
the last comparison follows already from $\pi>157/50$.
Consequently
\[
\Delta_{n,p,k}(n+2)\beta_p^2
<\left(\frac{807}{2000}\right)^2\frac{16}{15}
=\frac{217083}{1250000}<\frac{87}{500}.
\]
For $26\le n\le31$, monotonicity reduces the comparison to the six
pairs in the table. Write $e=\varepsilon^2$.
The fourth column is $10^9\alpha$, where
$\alpha^2>e(1+e)/14$.
The last column gives a strict rational upper bound $U$ for
$\Delta_{n,p,k}(n+2)\beta_p^2$.
Every terminating decimal in this table is exact.
\begin{center}
\begin{tabular}{@{}ccccc@{}}
\toprule
$n$&$p$&$e$&$10^9\alpha$&$U$\\
\midrule
26&18&$11/540$&38531363&0.173413\\
27&19&$11/589$&36863168&0.164766\\
28&19&$3/152$&37915682&0.173793\\
29&20&$1/55$&36363637&0.165557\\
30&20&$13/680$&37304856&0.173910\\
31&21&$13/735$&35856767&0.166064\\
\bottomrule
\end{tabular}
\end{center}
All entries are certified by rational inequalities.
Here are complete instructions for checking every entry.
For $p=2m+1$ use the exact value
$\beta_p=\binom{2m}{m}/4^m$.
For $p=2m$ use
\[
\beta_p=\frac{4^m m!(m-1)!}{\pi(2m)!},
\qquad \pi>\frac{314159}{100000},
\]
to obtain a rational strict upper bound $B_p$ for $\beta_p^2$.
For odd $p$, set $B_p=\beta_p^2$.
Squaring the indicated rational $\alpha$ verifies its claimed bound.
Substitution then gives, in each row,
\[
(n+2)B_p\left(e+\frac{1+e}{14}+2\alpha\right)