\documentclass[11pt]{article} \usepackage[T1]{fontenc} \usepackage[margin=1in]{geometry} \usepackage{amsmath,amssymb,amsthm,mathtools,mathrsfs} \usepackage{tikz} \usetikzlibrary{decorations.markings} \usepackage[colorlinks=true,linkcolor=blue,citecolor=blue,urlcolor=blue]{hyperref} \emergencystretch=1.5em \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{\norm}[1]{\left\lVert #1\right\rVert} \newcommand{\Id}{\mathrm{Id}} \newcommand{\Mom}{\mathsf M} \newcommand{\Aminus}{A_-} \newcommand{\Aplus}{A_+} \newcommand{\cuspq}{\mathfrak q} \newcommand{\SL}{\mathrm{SL}_2(\mathbb Z)} \newcommand{\PSL}{\mathrm{PSL}_2(\mathbb Z)} \DeclareMathOperator{\ord}{ord} \title{A construction of the sphere-packing magic functions in dimensions 8 and 24} \author{} \date{} \begin{document} \maketitle \begin{abstract} We develop an alternative route to the solutions of the sphere-packing problem in dimensions \(8\) and \(24\), through the auxiliary functions in the Cohn--Elkies Fourier bound. In each dimension we construct a radial Schwartz function with the prescribed lattice zeros by solving a countable system of linear equations in absolutely summable coefficients. We prove existence and uniqueness after normalization, without using the known magic functions or Fourier interpolation. Through a Cauchy boundary problem, solutions of the homogeneous equations are identified with global sections of a rank-six holomorphic vector bundle over the compactified modular curve of the full modular group, with its orbifold structure retained. Riemann--Roch shows that this bundle has Euler characteristic one, forcing a nonzero global section and hence a nontrivial solution of the equations. A separate argument proves uniqueness after normalization. An equivalent positive operator equation has a bounded inverse. The construction is motivated by the coefficient method for planar circle packing. A subsequent comparison identifies our solutions with the functions of Viazovska and of Cohn, Kumar, Miller, Radchenko, and Viazovska. The route to sphere packing is not yet independent in its entirety: we do not prove the required global sign inequalities from the coefficient equations. Those inequalities are inherited from the known functions after identification. \end{abstract} \section{Introduction} The Fourier bound of Cohn and Elkies \cite{CE} converts sphere packing into a problem about a function and its Fourier transform. A suitable auxiliary function gives an upper bound on the density of every packing. In dimensions \(8\) and \(24\), specially chosen functions make this bound equal to the densities of the \(E_8\) and Leech lattices, respectively, and hence prove their optimality. Such sharp auxiliary functions are often called \emph{magic functions}. This paper gives a construction of those functions from countably many linear equations. There are two distinct tasks in a sharp Fourier bound: constructing the function with the required zeros and normalization, and proving its signs between those zeros. We give existence and uniqueness proofs for the coefficient systems in both dimensions. We then identify the resulting functions with the known magic functions. We do not give independent proofs of the global sign inequalities. Thus the construction part is independent of the earlier magic functions, but a complete sphere-packing proof still uses their established signs. Section~\ref{sec:signs} describes this remaining task and the methods used to address it in the planar case. \subsection{The functions to be constructed} Fix \(d\in\{8,24\}\). Let \(\mathbf y,\boldsymbol{\xi}\in\mathbb R^d\) denote a spatial vector and a frequency vector, respectively. For a Schwartz function \(f:\mathbb R^d\to\mathbb C\), define \begin{equation} \widehat f(\boldsymbol{\xi})=\int_{\mathbb R^d} f(\mathbf y)e^{-2\pi i \mathbf y\cdot\boldsymbol{\xi}}\,d\mathbf y. \label{eq:Fourier-convention} \end{equation} Here \(\mathbf y\cdot\boldsymbol{\xi}\) is the Euclidean inner product. A Schwartz function is smooth and, together with each derivative, decays faster than every inverse power of \(|\mathbf y|\). We consider radial functions: \(f(\mathbf y)\) depends only on \(|\mathbf y|\). Their Fourier transforms are radial as well. For a radial \(f\), define \(\Phi,G:[0,\infty)\to\mathbb C\) by \begin{equation} f(\mathbf y)=\Phi(|\mathbf y|^2),\qquad \widehat f(\boldsymbol{\xi})=G(|\boldsymbol{\xi}|^2). \label{eq:radial-profiles} \end{equation} The letters \(u,v\) denote independent real arguments in \([0,\infty)\) of \(\Phi,G\), respectively. In the displayed identities we evaluate these functions at \(|\mathbf y|^2,|\boldsymbol{\xi}|^2\). Primes denote ordinary derivatives of the one-variable functions; in particular \(\frac{d}{dr}\Phi(r^2)=2r\Phi'(r^2)\). Put \(n_8=1\) and \(n_{24}=2\). In the normalization where each lattice has covolume one, its first nonzero squared length is \(2n_d\). The Cohn--Elkies bound asks for a real radial Schwartz function satisfying \begin{equation} \Phi(0)=G(0)=1,\qquad \Phi(u)\leq0\quad(u\geq2n_d),\qquad G(v)\geq0\quad(v\geq0). \label{eq:sign-goal} \end{equation} It then bounds the packing density by the volume of a ball of radius \(\sqrt{2n_d}/2\), which is precisely the density of the corresponding lattice packing. The lattices are even, so their nonzero squared lengths belong to \(2\mathbb Z\), starting at \(2n_d\); see \cite[Section 1]{V} and \cite[Section 1]{CKMRV24}. Equality in the Fourier bound forces both profiles to vanish at the lattice lengths. We impose these conditions at every node \(2n\), \(n\geq n_d\). The sign inequalities also force their derivatives to vanish, except possibly at the first zero of \(\Phi\), the endpoint of its required sign interval. The equalities to be imposed are therefore \begin{align} \Phi(2n)&=0 &&(n\geq n_d),& \Phi'(2n)&=0 &&(n>n_d),\nonumber\\ G(2n)&=0 &&(n\geq n_d),& G'(2n)&=0 &&(n\geq n_d). \label{eq:desired-zeros} \end{align} Our coefficient theorems construct normalized functions satisfying these equalities. From this point on, our proofs concern their construction and uniqueness; we do not return to an independent proof of the more general inequalities \eqref{eq:sign-goal}. The later comparisons with the known magic functions transfer the established signs to our solutions. There are well-documented methods for proving the required inequalities. Viazovska's original dimension-eight proof combines interval arithmetic with asymptotic expansions and rigorous remainder bounds near the two ends of the integral parameter range \cite[Section 5]{V}. In dimension \(24\), Cohn, Kumar, Miller, Radchenko, and Viazovska bound the errors in truncated Fourier series of modular forms and use Sturm's theorem for real polynomials, with exact rational arithmetic, to certify the remaining signs \cite[Appendix A]{CKMRV24}. Subsequent proofs replace these numerical certifications by structural arguments: Dan Romik proves the dimension-eight modular-form inequalities directly using modular identities, coefficient positivity, and special values \cite{Romik}; Seewoo Lee gives algebraic proofs in both dimensions using differential identities, positivity under Serre differentiation, and monotonicity of ratios of modular forms \cite[Sections 3, 5, and 6]{Lee}. The recent planar construction instead uses certified polynomial approximations in the Bernstein basis, together with coefficient error bounds and estimates for the unbounded region \cite[Section 4 and Appendices A--B]{OpenAI}. Section~\ref{sec:signs} describes that Bernstein approach and what would be needed to apply it to the present coefficient construction. \subsection{The planar construction as the starting point} The guiding method comes from the planar circle-packing preprint of OpenAI \cite[Sections 2, 3, and 5]{OpenAI}. That paper starts with a trigonometric polynomial having double zeros at a periodic set of nodes. Dividing by linear and quadratic factors permits changes to a value or first derivative at a chosen node. Gaussian damping turns these expressions into radial Schwartz functions. Their coefficients are determined by imposing Fourier conditions. Estimates on the entire coefficient space control the infinite system, and Poisson summation determines the normalization. We adopt this sequence of ideas: choose a family with the required zeros, express the Fourier conditions as linear equations, control the infinite coefficient space, and recover normalization by Poisson summation. In both dimensions studied here, the evenly spaced nodes allow the common factor \[ P(u)=\sin^2(\pi u/2). \] We combine it with integrals of Gaussians over \(t\geq1\) and \(0\ell\) they agree with the expressions obtained formally from \eqref{eq:U} at \(m=-\ell\), after the corresponding exponential rescaling. At \(u=\ell\) their singularities are removable, since \(P\) has a double zero. In particular, \[ \lim_{u\to0}\frac{R_{0,0}(u)}u=\frac{\pi}{4}, \qquad R_{0,1}(0)=\frac14. \] At the respective removable points one also has \[ R_{\ell,0}(\ell)=0,\qquad R_{\ell,0}'(\ell)=\frac{\pi}{4}, \qquad R_{\ell,1}(\ell)=\frac14,\qquad R_{\ell,1}'(\ell)=0. \] Thus the correction functions deliberately change the zero order; they are not included in the double-zero assertion for \(m\geq1\). A simple denominator permits a nonzero first derivative; a double denominator permits a nonzero value. These five functions therefore allow a value and a derivative at \(0\), a value and a derivative at \(2\), and a derivative at \(4\). All other zeros required of \(\Phi\) in \eqref{eq:desired-zeros} remain built into the family. The point \(2\) is allowed because the Leech lattice has no vectors of squared length \(2\). \subsection{Unknown coefficients and their norms} The coefficients are indexed by pairs \((j,m)\). The first subscript specifies a generating series and the second its exponent. Define the common set of positive-mode indices by \[ \mathcal I_+ =\bigl(\{0,1,2\}\times2\mathbb N\bigr) \cup\bigl(\{3\}\times(2\mathbb N-1)\bigr), \] and the dimension-24 indexing set by \[ \mathcal I_{24} =\{(0,-4),(0,-2),(0,0),(1,-2),(1,0)\}\cup\mathcal I_+. \] A coefficient vector is a family \(\mathbf c=(c_{j,m})_{(j,m)\in\mathcal I_{24}}\) of complex numbers. Its five nonpositive modes multiply the correction functions. Its positive modes give three sequences for even \(m\) and one for odd \(m\). This indexing will also be used in the generating series of Section~\ref{sec:boundary}. For \(p=1,2\), define the norm by \begin{align} \|\mathbf c\|_p^p={}& |c_{0,-4}|^p+|c_{0,-2}|^p+|c_{0,0}|^p +|c_{1,-2}|^p+|c_{1,0}|^p\nonumber\\ &+\sum_{m\in2\mathbb N}\sum_{k=0}^2|c_{k,m}|^p +\sum_{m\in2\mathbb N-1}|c_{3,m}|^p. \label{eq:coefficient-norm} \end{align} For \(p=1,2\), write \(\ell^p(\mathcal I_{24})\) for the space of these coefficient families with finite norm \(\|\mathbf c\|_p\). Thus \begin{align*} \ell^1(\mathcal I_{24})&=\mathbb C^5\oplus\ell^1(2\mathbb N)^3 \oplus\ell^1(2\mathbb N-1),\\ \ell^2(\mathcal I_{24})&=\mathbb C^5\oplus\ell^2(2\mathbb N)^3 \oplus\ell^2(2\mathbb N-1). \end{align*} We equip \(\ell^2(\mathcal I_{24})\) with its standard coefficient inner product associated with the sum in \eqref{eq:coefficient-norm}. Every sequence space below displays its indexing set. Lebesgue spaces of functions, used later for boundary values, are denoted by \(L^p\). The construction seeks a vector in \(\ell^1(\mathcal I_{24})\). Working temporarily in the larger Hilbert space \(\ell^2(\mathcal I_{24})\) permits the use of adjoints and compact operators. We will prove that every exact solution in \(\ell^2(\mathcal I_{24})\) already belongs to \(\ell^1(\mathcal I_{24})\). For \(\mathbf c\in\ell^2(\mathcal I_{24})\), define a function \(\Phi_{\mathbf c}:[0,\infty)\to\mathbb C\) by the following series, with independent argument \(u\geq0\): \begin{align} \Phi_{\mathbf c}(u)={}& c_{1,0}R_{0,1}(u)+c_{0,0}R_{0,0}(u)\nonumber\\ &+e^{-2\pi}c_{1,-2}R_{2,1}(u) +e^{-2\pi}c_{0,-2}R_{2,0}(u) +e^{-4\pi}c_{0,-4}R_{4,0}(u)\nonumber\\ &+\sum_{m\in2\mathbb N-1}c_{3,m}\bigl(U_{m,0}(u)-2V_m(u)\bigr) \nonumber\\ &+\sum_{m\in2\mathbb N} \bigl(c_{0,m}U_{m,0}(u)+c_{1,m}U_{m,1}(u) +c_{2,m}(U_{m,2}(u)+V_m(u))\bigr). \label{eq:ansatz} \end{align} Lemma~\ref{lem:Schwartz} proves that this series defines a radial Schwartz function \[ f_{\mathbf c}(\mathbf y)=\Phi_{\mathbf c}(|\mathbf y|^2),\qquad \mathbf y\in\mathbb R^{24}. \] Using \eqref{eq:Fourier-convention}, let \(G_{\mathbf c}\) be the unique function on \([0,\infty)\) satisfying \[ \widehat f_{\mathbf c}(\boldsymbol{\xi})=G_{\mathbf c}(|\boldsymbol{\xi}|^2), \qquad \boldsymbol{\xi}\in\mathbb R^{24}. \] Thus \(\Phi_{\mathbf c}\) is specified by the coefficients, whereas \(G_{\mathbf c}\) is obtained from it by Fourier transformation. Both depend linearly on \(\mathbf c\). Only \(R_{0,1}\) in \eqref{eq:ansatz} is nonzero at \(u=0\), and \(R_{0,1}(0)=1/4\). It is therefore convenient to name the normalizing linear functional \begin{equation} \lambda(\mathbf c)=c_{1,0}/4=\Phi_{\mathbf c}(0). \label{eq:lambda} \end{equation} \subsection{The equations and the main theorem} The required zeros of \(\Phi_{\mathbf c}\) are automatic from the choice of functions. The unknown coefficients must make the Fourier profile satisfy \begin{equation} G_{\mathbf c}(2n)=G_{\mathbf c}'(2n)=0\quad(n\geq2), \qquad \lambda(\mathbf c)=1. \label{eq:system} \end{equation} Here is the linear system explicitly. In this paragraph only, enumerate the entries of \(\mathbf c\) by \(j\in\mathbb N\), write \(c_j\) for the corresponding scalar, and let \(\mathbf e_j\) be the coefficient family with that entry equal to one and all other entries zero. Put \(g_j=G_{\mathbf e_j}\); these are fixed functions, obtained by Fourier transforming the individual terms of \eqref{eq:ansatz}. The equations are \begin{equation} \begin{gathered} \sum_{j\geq1}g_j(2n)c_j=0,\qquad \sum_{j\geq1}g_j'(2n)c_j=0\quad(n\geq2),\\ \sum_{j\geq1}\lambda(\mathbf e_j)c_j=1. \end{gathered} \label{eq:matrix-system} \end{equation} Thus \(g_j(2n)\) and \(g_j'(2n)\) are matrix entries, not unknowns. Only the \(c_j\) are unknown. The last row has a single nonzero entry, \(1/4\), in the position of \(c_{1,0}\). Lemma~\ref{lem:Schwartz} justifies the series and evaluation term by term. Lemma~\ref{lem:samples} will express the two types of Fourier rows as contour integrals. \begin{theorem}[Coefficient construction]\label{thm:main} The system \eqref{eq:system} has exactly one solution \(\mathbf c_*\) in \(\ell^2(\mathcal I_{24})\). Its entries are real, and it belongs to \(\ell^1(\mathcal I_{24})\). More precisely, for every \(10\), apply Poisson summation to \(\mathbf y\mapsto f_{\mathbf c}(\sqrt t\,\mathbf y)\): \[ \Phi_{\mathbf c}(0)+\sum_{n\geq2}N_n\Phi_{\mathbf c}(2nt) =t^{-12}\left(G_{\mathbf c}(0)+\sum_{n\geq2}N_nG_{\mathbf c}(2n/t)\right). \] Schwartz regularity justifies differentiation locally uniformly in \(t>0\). Evaluate at \(t=1\), and then differentiate and evaluate there, using \eqref{eq:physical-jets}. The identities follow; \(N_2/12=16380\) gives \eqref{eq:normalizations}. \end{proof} \section{From Fourier samples to a boundary problem}\label{sec:boundary} This section replaces the Fourier equations by a problem in one complex variable. Its first objective is the following identity. The measures in the statement are defined explicitly in \eqref{eq:measures}; their supports are independent of the coefficient vector. Their dependence on that vector is linear. \begin{lemma}[Fourier samples as contour integrals]\label{lem:samples} For each \(\mathbf c\in\ell^2(\mathcal I_{24})\), let \(\mu_0,\mu_1\) be the finite complex measures constructed in \eqref{eq:measures}. For every integer \(n\geq0\), \begin{equation} G_{\mathbf c}(2n)=\frac1{8\pi}\int_{\mathbb C}w^{n-1}\,d\mu_0(w),\qquad G_{\mathbf c}'(2n)=-\frac18\int_{\mathbb C}w^{n-1}\,d\mu_1(w). \label{eq:samples} \end{equation} The integrals converge absolutely, including when \(n=0\). \end{lemma} Thus the equations for \(n\geq2\) are exactly the vanishing of the moments of positive degree of these measures. Once the lemma has been proved, we package the moments as an operator and use Cauchy integrals to express their vanishing as boundary conditions for holomorphic functions. \subsection{Gaussian parameters and generating series} For each fixed \(z\in\mathbb C\) with \(\Re z>0\), define \(g_z(\mathbf y)=e^{-\pi z|\mathbf y|^2}\), \(\mathbf y\in\mathbb R^{24}\). Gaussian Fourier inversion gives, for every fixed \(\boldsymbol{\xi}\in\mathbb R^{24}\), \begin{equation} \widehat g_z(\boldsymbol{\xi}) =\int_{\mathbb R^{24}}e^{-\pi z|\mathbf y|^2}e^{-2\pi i \mathbf y\cdot\boldsymbol{\xi}}\,d\mathbf y =z^{-12}e^{-\pi|\boldsymbol{\xi}|^2/z}. \label{eq:Gaussian} \end{equation} Only \(\mathbf y\) is integrated in this formula. Equivalently, the one-variable function giving its radial Fourier values is \(v\mapsto z^{-12}e^{-\pi v/z}\), for an independent real argument \(v\geq0\). In the contour calculations below we hold \(v\) fixed and integrate in \(z\). We then evaluate at \(v=2n\), or differentiate with respect to \(v\) and evaluate there. No frequency vector \(\boldsymbol{\xi}\) occurs in those calculations. Define two maps, with different roles: \begin{equation} Q(z)=e^{-\pi(z-1)}\quad(z\in\mathbb C),\qquad \omega(z)=e^{-2\pi/z}\quad(z\in\mathbb C\setminus\{0\}). \label{eq:parameter-maps} \end{equation} The map \(Q\) supplies arguments for generating series; the map \(\omega\) supplies points of the contour plane. In particular \(e^{-\pi(2n)/z}=\omega(z)^n\), which is the source of the powers in \eqref{eq:samples}. We reserve \(q\) for an independent complex argument of a generating series and \(w\) for an independent complex coordinate in the contour plane. Neither letter denotes a map. Fix \(\mathbf c\in\ell^2(\mathcal I_{24})\) for the definitions that follow. All generating series, densities, and measures depend on this fixed vector; we omit that dependence from their subscripts. For \(0<|q|<1\), define \begin{align} A_0(q)&=c_{0,-4}q^{-4}+c_{0,-2}q^{-2}+c_{0,0} +\sum_{m\in2\mathbb N}c_{0,m}q^m,\nonumber\\ A_1(q)&=c_{1,-2}q^{-2}+c_{1,0} +\sum_{m\in2\mathbb N}c_{1,m}q^m,\nonumber\\ A_2(q)&=\sum_{m\in2\mathbb N}c_{2,m}q^m,\nonumber\\ A_3(q)&=\sum_{m\in2\mathbb N-1}c_{3,m}q^m. \label{eq:series} \end{align} These series already contain four of the six functions that will represent a global section of the bundle. More precisely, for a complex variable \(\tau\) with \(\Im\tau>1\), substitute \(q=Q(-i\tau)=e^\pi e^{\pi i\tau}\) and form \[ \bigl(A_0(q),-iA_1(q),-A_2(q),A_3(q)\bigr). \] When the Fourier equations are satisfied, these four functions continue holomorphically to the upper half-plane and become the first four components of a section of the rank-six bundle over the compactified modular curve, with the orbifold and cusp conditions described in Section~\ref{sec:bundle}. The other two components come from the Cauchy integrals. This assertion is proved in Proposition~\ref{prop:equivalence}; it is not an additional assumption on the series. The components are coordinate functions of a bundle section, rather than four separately invariant functions on the modular curve. Set \(A_-(q)=A_2(q)-2A_3(q)\) and \(A_+(q)=A_2(q)+2A_3(q)\). The first three series are even functions of \(q\); the fourth is odd. Define, for \(\Re z>1\), \begin{align} b_0(z)&=A_0(Q(z))+zA_1(Q(z))+z^2A_2(Q(z))+A_3(Q(z)),\nonumber\\ b_1(z)&=A_1(Q(z))+2zA_2(Q(z)). \label{eq:BL} \end{align} These evaluations are within the convergence disk because \(|Q(z)|<1\) precisely when \(\Re z>1\). We also need values on the line \(\Re z=1\). They are initially boundary limits, not values of a continuation already known to exist. Indeed, \(Q(\sigma+it)=e^{-\pi(\sigma-1)}e^{-\pi it}\). As \(\sigma\downarrow1\), square summability and Parseval's identity give convergence in \(L^2\) on bounded \(t\)-intervals of each series and of \(b_0,b_1\). These \(L^2\) limits are called \emph{boundary traces}. Evaluations of these functions on \(\Re z=1\) below mean these traces, defined almost everywhere. \subsection{The parametrized contours and the measures} Define paths in the Gaussian-parameter plane by \[ z_+(t)=1+it,\qquad z_-(t)=1-i+it,\qquad 0\leq t\leq1, \] and paths in the contour plane by \[ \gamma_+(t)=\omega(z_+(t)),\qquad \gamma_-(t)=\omega(z_-(t)),\qquad 0\leq t\leq1. \] Put \(w_0=e^{-2\pi}\) and \(w_c=-e^{-\pi}\). As \(t\) increases, \(\gamma_+\) runs from \(w_0\) to \(w_c\) in the upper half-plane, and \(\gamma_-\) runs from \(w_c\) to \(w_0\) in the lower half-plane. Explicitly, \(\gamma_-(t)=\overline{\gamma_+(1-t)}\); this formula specifies the reversal of direction in the conjugate path. Let \(\Gamma_\pm=\gamma_\pm([0,1])\) be their images, and let \(\Gamma=\Gamma_+\cup\Gamma_-\) be the resulting set. The set \(\Gamma\) is a Jordan curve. For example, along \(\gamma_+\) the argument \(2\pi t/(1+t^2)\) increases from \(0\) to \(\pi\), which proves simplicity on that half. Let \(\Omega\) be the bounded component of \(\mathbb C\setminus\Gamma\). It contains \(0\). Traversing \(\gamma_+\) followed by \(\gamma_-\) gives the positive orientation of its boundary. Whenever we integrate over \(\Gamma\), we mean the sum of the integrals along these two parametrized paths. The two analytic arcs meet tangentially at \(w_c\), with the direction of traversal reversing along their common tangent. This is the nonsmooth point of the Jordan curve, called its \emph{contour cusp} below. The curve is smooth at \(w_0\), but an additional segment will meet it there. Set \(I=(0,w_0)\subset\mathbb R\). Integrals along this segment use the path \(s\mapsto s\), \(0=latex,font=\small] % A uniform enlargement by exp(pi) preserves the contour's shape. \coordinate (wc) at (-1,0); \coordinate (wzero) at ({exp(-pi)},0); \coordinate (origin) at (0,0); \draw[gray!55,thin,->] (-1.065,0)--(.235,0) node[right,black] {$\Re w$}; \draw[gray!55,thin,->] (0,-.135)--(0,.155) node[above,black] {$\Im w$}; \draw[thick,postaction={decorate}, decoration={markings,mark=at position .55 with {\arrow{>}}}] plot[domain=0:1,samples=201,variable=\t] ({exp(pi-2*pi/(1+\t*\t))*cos(360*\t/(1+\t*\t))}, {exp(pi-2*pi/(1+\t*\t))*sin(360*\t/(1+\t*\t))}); \draw[thick,postaction={decorate}, decoration={markings,mark=at position .45 with {\arrow{>}}}] plot[domain=1:0,samples=201,variable=\t] ({exp(pi-2*pi/(1+\t*\t))*cos(360*\t/(1+\t*\t))}, {-exp(pi-2*pi/(1+\t*\t))*sin(360*\t/(1+\t*\t))}); \draw[very thick,->] (origin)--(wzero); \node at (-.16,.116) {$\Gamma_+$}; \node at (-.16,-.116) {$\Gamma_-$}; \node at (-.36,0) [fill=white,inner sep=2pt] {$\Omega$}; \fill (wc) circle[radius=1.1pt]; \fill (origin) circle[radius=1.1pt]; \fill (wzero) circle[radius=1.1pt]; \node[below=5pt] at (wc) {$w_c=-e^{-\pi}$}; \node[below left=3pt] at (origin) {$0$}; \draw[thin] (wzero)--(.09,.065) node[right] {$w_0=e^{-2\pi}$}; \draw[thin] ({exp(-pi)/2},0)--(.09,-.065) node[right] {$I=(0,w_0)$}; \end{tikzpicture} \caption{The contour \(\Gamma=\Gamma_+\cup\Gamma_-\) and the segment \(I\), drawn with a uniform enlargement. The upper arc runs from \(w_0\) to \(w_c\), the lower arc returns to \(w_0\), and \(I\) is directed from \(0\) towards \(w_0\). The arcs meet tangentially at the cusp \(w_c\).} \label{fig:contour} \end{figure} Define the boundary densities \(\rho_{0,\Gamma},\rho_{1,\Gamma}\) almost everywhere on \(\Gamma\) by the following four formulas. Every occurrence of \(b_0,b_1,A_j,A_\pm\) has its argument displayed: \begin{align} \rho_{0,\Gamma}(\gamma_+(t)) &=z_+(t)^{-10}\bigl[b_0(z_+(t))-ib_1(z_+(t))\bigr],\nonumber\\ \rho_{1,\Gamma}(\gamma_+(t)) &=z_+(t)^{-11}\bigl[b_0(z_+(t))-ib_1(z_+(t)) +iz_+(t)A_+(Q(z_+(t)))\bigr],\nonumber\\ \rho_{0,\Gamma}(\gamma_-(t)) &=-z_-(t)^{-10}\bigl[b_0(z_-(t))+ib_1(z_-(t))\bigr],\nonumber\\ \rho_{1,\Gamma}(\gamma_-(t)) &=-z_-(t)^{-11}\bigl[b_0(z_-(t))+ib_1(z_-(t)) -iz_-(t)A_+(Q(z_-(t)))\bigr]. \label{eq:densities} \end{align} Here \(0J. \end{cases} \] Here \(\mathbf b=(b_{\nu,k})\in\ell^2(\mathcal J_{24})\). This projection has rank \(2J\). The same geometric estimate gives \begin{equation} \|(\Id_{\mathcal J_{24}}-\mathsf Q_J)\Mom\|\leq C_\mu\frac{\rho^{J+1}}{\sqrt{1-\rho^2}}. \label{eq:Acompact} \end{equation} Thus \(\Mom\) is a compact linear operator: the finite-rank operators \(\mathsf Q_J\Mom\) converge to it in operator norm. This compactness is useful, but is not an existence theorem for the normalized equations. The continuation and index arguments below supply existence. \subsection{Cauchy functions, traces, and jumps}\label{sec:traces} Fix \(\mathbf c\in\ell^2(\mathcal I_{24})\), and form its measures and their zeroth moments as above. For an evaluation point \(\zeta\in\mathbb C\setminus(\Gamma\cup[0,w_0])\), define \begin{equation} h_\nu(\zeta)=\frac1{2\pi i} \left(\int_{\mathbb C}\frac{d\mu_\nu(w)}{w-\zeta} +\frac{m_{\nu,0}}{\zeta}\right),\qquad \nu=0,1. \label{eq:Cauchy} \end{equation} We call these the \emph{corrected Cauchy transforms}, or \emph{Cauchy functions}, of the coefficient vector. In this integral \(\zeta\) is fixed and \(w\) is integrated. The correction term removes the zeroth moment from the expansion at infinity. Write \(\mathbf h=(h_0,h_1)^T\). If \(\mathbf c\in\ker\Mom\), then for \(|\zeta|>\rho\) the convergent expansion of \((w-\zeta)^{-1}\) gives \[ \int_{\mathbb C}\frac{d\mu_\nu(w)}{w-\zeta} =-\sum_{k\geq0}\zeta^{-k-1} \int_{\mathbb C}w^k\,d\mu_\nu(w) =-m_{\nu,0}/\zeta. \] Hence \(h_\nu=0\) on the unbounded component of \(\mathbb C\setminus\Gamma\), by analytic continuation. Inside \(\Omega\), it is holomorphic away from the closed segment \([0,w_0]\). Removing that segment gives a \emph{slit domain}. At a point \(s\in I\) there are two boundary approaches within this domain: from above and from below the real axis. We denote their traces by \(h_{\nu,+}(s)\) and \(h_{\nu,-}(s)\). On \(\Gamma\), the interior trace is the limit approached from \(\Omega\); the exterior trace is approached from the unbounded component. All assertions about these limits are local on open arcs away from \(0,w_0,w_c\). More precisely, after straightening an arc by a holomorphic coordinate, the restrictions to parallel lines converge in \(L^2\) on every smaller closed interval. We use this meaning of local \(L^2\) trace convergence throughout. The limits also exist almost everywhere in the nontangential sense. A nontangential approach stays inside a cone that makes a positive angle with the boundary tangent. The Cauchy jump formula then gives \begin{align} h_{\nu,\mathrm{int}}(w)&=\rho_{\nu,\Gamma}(w) &&(w\in\Gamma\setminus\{w_0,w_c\}),\nonumber\\ h_{0,+}(s)-h_{0,-}(s) &=2A_-(e^\pi\sqrt s) &&(s\in I),\nonumber\\ h_{1,+}(s)-h_{1,-}(s) &=-\pi^{-1}(\log s)\,A_-(e^\pi\sqrt s) &&(s\in I). \label{eq:jumps} \end{align} The first line uses the zero exterior trace. The next two give the jump, meaning the upper trace minus the lower trace, across the segment oriented towards \(w_0\). For clarity, we recall the analytic facts used here. On the real line directed from left to right, the Cauchy integral of \(g\in L^2(\mathbb R)\) is \[ (\mathsf Cg)(\zeta)=\frac1{2\pi i}\int_{\mathbb R} \frac{g(x)}{x-\zeta}\,dx, \qquad \Im\zeta\ne0. \] Its upper and lower traces are \(\mathsf C_+g=\mathsf P_+g\) and \(\mathsf C_-g=-\mathsf P_-g\), where \(\mathsf P_\pm\) are the orthogonal projections onto the subspaces with Fourier transform supported in the positive and negative half-lines. They are called \emph{Hardy projections}. Their ranges are the boundary values of the Hardy spaces: holomorphic functions on the respective half-planes whose squared integrals along horizontal lines are uniformly bounded. Thus \(\mathsf C_+-\mathsf C_-=\mathsf P_++\mathsf P_-=\Id_{L^2(\mathbb R)}\). See \cite[Sections 8.2--8.3 and 8.7]{Srivastava} for the boundary-value description and Cauchy representation. For an open analytic arc, choose a smaller subarc, cut off the density outside a slightly larger subarc, and straighten the arc by a holomorphic coordinate. The transformed Cauchy kernel differs from the real-line kernel by a bounded smooth kernel; the omitted part of the contour contributes a holomorphic function near the smaller subarc. The real-line result therefore proves the local \(L^2\) trace and jump statements used in \eqref{eq:jumps}. This is the local form of the Plemelj formula; see \cite[Section 3.5, especially (3.5.3)--(3.5.5)]{Trogdon}. No trace theorem at the nonsmooth point \(w_c\) is being invoked. \begin{lemma}[Gluing across an open arc]\label{lem:trace-gluing} Let an analytic arc divide a neighborhood into two sides, and let \(h_+,h_-\) be holomorphic on those sides. Suppose their traces converge locally in \(L^2\), in the sense just specified, to the same function. Then they are restrictions of one holomorphic function on a neighborhood of the open arc. \end{lemma} \begin{proof} Straighten the arc and restrict to a smaller rectangle. Trace convergence bounds the \(L^2\) norms on parallel intervals uniformly near the real axis. Cauchy--Schwarz followed by integration in the perpendicular coordinate gives local area integrability of the function \(h_{\mathrm{glue}}\) defined by the two pieces. For a smooth compactly supported test function, integrate by parts above the line of height \(r\) and below the line of height \(-r\). Holomorphy leaves only the two boundary terms. Their difference tends to zero by \(L^2\) trace convergence, so \(\bar\partial h_{\mathrm{glue}}=0\) in distributions. Local convolution with a smooth approximate identity gives holomorphic functions converging to \(h_{\mathrm{glue}}\) in local \(L^1\). The area mean inequality makes this convergence uniform on smaller disks. Its limit is the required extension. \end{proof} For continuous matching values this is also the consequence of Morera's theorem obtained by splitting triangles along the arc; see \cite[Section 1]{Zeff}. In our applications the original coefficient series have the asserted trace convergence by the Hardy-space theorem, and the Cauchy functions have it by the localized Plemelj formula above. We require no trace theorem at a contour endpoint. \subsection{Reconstructing the equations from boundary data} We have proved that a coefficient solution gives holomorphic Cauchy functions with the boundary conditions \eqref{eq:jumps}. The reverse implication, needed for the existence proof, is the following statement. Its endpoint assumptions prevent additional singular terms that the jumps on open arcs cannot detect. For \(\zeta_0\in\mathbb C\) and \(r>0\), write \(D(\zeta_0,r)=\{w:|w-\zeta_0|1\) lies in the half-plane where the coefficient series already converge. \subsection{Area bounds and removal of a puncture} We record the estimates before constructing any continuation. They apply to arbitrary coefficient vectors; matching traces will be used only when constructing a solution's holomorphic extension. Throughout this section \(dA\) denotes ordinary planar area. \begin{lemma}[Local area estimates]\label{lem:local-area} For a bounded measurable set \(E\) whose closure avoids zero, \[ \int_E|h_\nu(\zeta)|\,dA(\zeta) \leq C_E\|\mathbf c\|_2,\qquad \nu=0,1. \] The same assertion holds for the compositions used below on fixed coordinate neighborhoods, provided the coordinate maps are one-to-one with nonzero derivatives and have images avoiding zero. For each fixed \(01}} \sum_{j=0}^3|A_j(Q(z))|\,dA(z)\leq C_r\|\mathbf c\|_2 . \] \end{lemma} \begin{proof} For a finite measure \(\mu\), Tonelli's theorem and the layer-cake formula for the radially decreasing kernel give \[ \int_E\left|\int\frac{d\mu(w)}{w-\zeta}\right|dA(\zeta) \leq\|\mu\|_{\mathrm{TV}} \sup_w\int_E|w-\zeta|^{-1}dA(\zeta) \leq2\sqrt{\pi\,\operatorname{area}(E)}\,\|\mu\|_{\mathrm{TV}}. \] The correction term \(m_{\nu,0}/\zeta\) has the required bound because \(E\) avoids zero. Use \eqref{eq:TV} to obtain the first assertion. Changes of variables with bounded Jacobian and bounded multipliers give the assertion about compositions. One may split a fixed neighborhood into finitely many coordinate patches when necessary. Writing \(x=\Re z-1>0\), Cauchy--Schwarz gives \begin{equation} \left|\sum_{m\geq1}\beta_m e^{-\pi m(z-1)}\right| \leq\frac{\|\boldsymbol\beta\|_2}{\sqrt{e^{2\pi x}-1}} \leq\frac{\|\boldsymbol\beta\|_2}{\sqrt{2\pi x}}. \label{eq:radial-series-bound} \end{equation} The finitely many nonpositive modes are uniformly bounded by \(C_r\|\mathbf c\|_2\) on this disk. Since \(x^{-1/2}\) is area-integrable on its right half, the last assertion follows. \end{proof} \begin{lemma}[Removal using one radius]\label{lem:area-removal} Let \(h\) be holomorphic and area-integrable on \(0<|z-z_0|1\) and \(C<\infty\), independent of \(\mathbf c\), such that every \(\mathbf c\in\ker_{\ell^2(\mathcal I_{24})}\Mom\) has \(q^4\mathbf a_{\mathrm{ser}}(q)\) holomorphic on a neighborhood of \(|q|\leq R\), and \begin{equation} \sup_{|q|=R}\|q^4\mathbf a_{\mathrm{ser}}(q)\|_1\leq C\|\mathbf c\|_2. \label{eq:regularity} \end{equation} In particular \(\ker_{\ell^2(\mathcal I_{24})}\Mom\subset\ell^1(\mathcal I_{24})\). \end{proposition} \begin{proof} \textit{The contour cusp.}\quad Use a local parameter \(z\) near \(1\); the arguments \(z+i,z-i\) approach the two ends of the contour at \(w_c=-e^{-\pi}\). Write \[ D_r=D(1,r),\qquad D_r^{\mathrm{out}}=D_r\cap\{|z|>1\},\qquad D_r^{\mathrm{in}}=D_r\cap\{|z|<1\}. \] Initially, on \(\Re z>1\), put \begin{align} b_{\mathrm{end}}(z)&=A_0(Q(z))+zA_1(Q(z)) +(z^2+1)A_2(Q(z))-A_3(Q(z)),\nonumber\\ b_-(z)&=\Aminus(Q(z)). \label{eq:localHX} \end{align} On the two portions of \(D_{1/4}^{\mathrm{out}}\) with \(\Re z<1\), define these two functions by solving \begin{align} \mathbf h_{\mathrm{par}}(z+i) &=\begin{pmatrix}b_{\mathrm{end}}(z)\\ b_{\mathrm{end}}(z)/(z+i)+ib_-(z)\end{pmatrix} &&(\Im z<0),\nonumber\\ \mathbf h_{\mathrm{par}}(z-i) &=\begin{pmatrix}-b_{\mathrm{end}}(z)\\ -b_{\mathrm{end}}(z)/(z-i)+ib_-(z)\end{pmatrix} &&(\Im z>0). \label{eq:local-lenses} \end{align} These are legitimate Cauchy evaluations. In the lower portion, \(|z|>1\) implies \(\Im z<-\sqrt{1-(\Re z)^2}\), so \(z+i\) lies in the upper half of \(\mathcal D\); the upper portion is analogous. The two equations are triangular and uniquely determine the two functions. On each open segment \(\Re z=1\), substitution of the outer densities, using the parity of \(A_j\), gives exactly the traces of \eqref{eq:localHX}. Lemma~\ref{lem:trace-gluing} therefore joins the three definitions into holomorphic functions on \(D_{1/4}^{\mathrm{out}}\). Lemma~\ref{lem:local-area} bounds their area norms there by \(C\|\mathbf c\|_2\): it covers both the original-series portion and the two Cauchy portions. All denominators \(z\pm i\) stay away from zero. On the two open arcs \(|z|=1\), \(z\ne1\), the circle matching law \eqref{eq:circle-transfer} yields \begin{equation} b_{\mathrm{end}}(z)=z^{10}b_{\mathrm{end}}(1/z),\qquad b_-(z)+z^{10}b_-(1/z)=b_{\mathrm{end}}(z). \label{eq:local-involution} \end{equation} Here is the algebra at the lower arc. The two arguments in \eqref{eq:local-lenses} are \(z+i\) and \(1/z-i\). Their circle-transfer multiplier is \((iz)^{10}=-z^{10}\). The first component gives the first identity, and the second gives the second, using \((1/z-i)^{-1}-(z+i)^{-1}=i\). The upper arc gives the inverse identities. These identities hold for the analytic germs at the open arcs, because their Cauchy arguments lie on the interior negative real interval of \(\Omega\), across which \(\mathbf h\) is holomorphic. For \(z\in D_{1/8}^{\mathrm{in}}\) define \[ b_{\mathrm{end}}(z)=z^{10}b_{\mathrm{end}}(1/z),\qquad b_-(z)=b_{\mathrm{end}}(z)-z^{10}b_-(1/z). \] The right sides have already been defined: \(|1/z|>1\) and \[ |1/z-1|\leq\frac{|z-1|}{1-|z-1|}<\frac17<\frac14. \] The transformation on the ordered pair is \(z^{10}\) times \(\left(\begin{smallmatrix}1&0\\1&-1\end{smallmatrix}\right)\); applying it at \(z\) and then \(1/z\) is the identity. The arc identities just proved match these inner pieces to the outer pieces. We thus have a single holomorphic pair on the whole punctured disk \(D_{1/8}\setminus\{1\}\). This specifies both the cover and all its overlaps. Inversion has bounded Jacobian on these disks, and \(z^{10}\) is bounded there. Lemma~\ref{lem:local-area} consequently bounds the area norm of the whole pair, including the inner pieces. On the radius \(z=1+t\), \eqref{eq:radial-series-bound} bounds each component by \(C\|\mathbf c\|_2(1+t^{-1/2})\). Lemma~\ref{lem:area-removal} removes both punctures and gives uniform bounds on \(D_{1/16}\). The involution identities continue wherever both sides are defined. In particular, \(b_-\) continues \(\Aminus(Q(z))\) through \(z=1\). \textit{The real endpoint and the remaining components.}\quad At the other contour endpoint \(w_0=e^{-2\pi}\), which corresponds to \(z=1\), define on the left of \(z=1\) \begin{equation} b_+(z)=-i\bigl(h_{1,\mathrm{par}}(z)-h_{0,\mathrm{par}}(z)/z\bigr). \label{eq:localXplus} \end{equation} Use this formula separately on the upper and lower left half-disks of \(D_{1/8}\), both contained in the corresponding halves of \(\mathcal D\). Its real-interval jump is zero: the jump vector in \eqref{eq:real-transfer} has second component equal to its first divided by \(z\). On the right half-disk use \(b_+(z)=\Aplus(Q(z))\). The outer trace formulas give this same value on the two open vertical segments. Applying Lemma~\ref{lem:trace-gluing} to the real interval and the vertical segments yields a holomorphic function on \(D_{1/8}\setminus\{1\}\). Its left pieces have the Cauchy area bound and its right piece has the series area bound of Lemma~\ref{lem:local-area}. On \(z=1+t\) it satisfies \eqref{eq:radial-series-bound}. Lemma~\ref{lem:area-removal} removes the puncture and bounds the extension on \(D_{1/16}\). Consequently \[ A_2(Q(z))=(b_+(z)+b_-(z))/2,\qquad A_3(Q(z))=(b_+(z)-b_-(z))/4 \] are holomorphic near that point. It remains to recover \(A_1,A_0\). Work on \(D_{1/32}\), where all three functions just constructed are bounded by \(C\|\mathbf c\|_2\). In the upper and lower left half-disks, the subscripts \(+\) and \(-\) on \(h_{0,\mathrm{par}}\) designate its holomorphic restrictions to those half-disks; on the intervening real interval they designate the corresponding traces. Use, respectively, \begin{align} A_1(Q(z))&=i\bigl[h_{0,\mathrm{par},+}(z)-b_{\mathrm{end}}(z) +(1+2iz)A_2(Q(z))-2A_3(Q(z))\bigr],\nonumber\\ A_1(Q(z))&=i\bigl[h_{0,\mathrm{par},-}(z)+b_{\mathrm{end}}(z) -(1-2iz)A_2(Q(z))+2A_3(Q(z))\bigr]. \label{eq:localA1} \end{align} Their difference is \(i[h_{0,\mathrm{par},+}(z)-h_{0,\mathrm{par},-}(z)-2b_{\mathrm{end}}(z)+2b_-(z)]\). On the real interval, \eqref{eq:real-transfer} identifies the jump of \(h_{0,\mathrm{par}}\) with \(2z^{10}b_-(1/z)\). The second identity of \eqref{eq:local-involution} identifies this with \(2b_{\mathrm{end}}(z)-2b_-(z)\). The difference is therefore zero. On \(\Re z=1\), direct substitution of the outer traces gives \(A_1(Q(z))\) from either formula. Glue the two left pieces to that original right-hand piece by Lemma~\ref{lem:trace-gluing}. Their area norms are bounded: use Lemma~\ref{lem:local-area} for the Cauchy terms and the original series, and the bounds on \(D_{1/32}\) for the other terms. The right-hand radius again satisfies \eqref{eq:radial-series-bound}. Lemma~\ref{lem:area-removal} now removes the puncture and bounds \(A_1(Q(z))\) on \(D_{1/64}\). Finally, \begin{equation} A_0(Q(z))=b_{\mathrm{end}}(z)-zA_1(Q(z))-(z^2+1)A_2(Q(z))+A_3(Q(z)). \label{eq:localA0} \end{equation} This formula agrees with the original \(A_0(Q(z))\) on the right half-disk by its definition in \eqref{eq:localHX}; it is holomorphic throughout \(D_{1/32}\) and bounded on \(D_{1/64}\). All four functions now extend across \(q=1\), and parity gives the same conclusion at \(q=-1\). \textit{A common annulus and its norm bound.}\quad For an explicit common neighborhood, put \(\delta_{\mathrm{strip}}=2^{-18}\) and \(\delta_{\mathrm{end}}=2^{-7}\). If \(1-\delta_{\mathrm{strip}}<\Re z<1\) and \(\delta_{\mathrm{end}}\leq\Im z\leq1-\delta_{\mathrm{end}}\), both \(z,z-i\) lie in the required halves of \(\mathcal D\), since \((1-\delta_{\mathrm{strip}})^2>1-\delta_{\mathrm{end}}^2\). Use \(\mathsf S_{\mathrm{pair}}(z)^{-1}\) there and the endpoint disks elsewhere. Parity covers a full period. Hence \(q^4\mathbf a_{\mathrm{ser}}\) is holomorphic for \(|q|0\}\). The linear change of coordinate \(z\mapsto\tau=iz\) identifies the right half-plane in the \(z\)-plane with \(\mathbb H\). In this section \(\tau\) is an independent variable in \(\mathbb H\), and the corresponding Gaussian parameter is \(-i\tau\). The map \(Q\) satisfies \begin{equation} Q(-i\tau)=e^\pi e^{\pi i\tau}. \label{eq:coordinates} \end{equation} For \(\Im\tau>1\), define \begin{align*} a_0(\tau)&=A_0(Q(-i\tau)),&a_1(\tau)&=-iA_1(Q(-i\tau)),\\ a_2(\tau)&=-A_2(Q(-i\tau)),&a_3(\tau)&=A_3(Q(-i\tau)). \end{align*} The first three are periodic under \(\tau\mapsto\tau+1\); the fourth changes sign. The global problem seeks continuations of these four functions to all of \(\mathbb H\), together with two more holomorphic functions \(a_4,a_5\) that are periodic. To explain the additional functions, first suppose such global functions are given. Define the branch \[ \log_{\mathrm{cut}}w=\log|w|+i\arg w,\qquad 0<\arg w<2\pi, \] on \(\mathbb C\setminus[0,\infty)\). Its restriction to \(\Omega\setminus[0,w_0]\) is used throughout this construction. For \(w\) in that slit domain, put \(\tau_w=\log_{\mathrm{cut}}w/(2\pi i)\). The upper and lower traces on the positive real segment use arguments \(0\) and \(2\pi\), respectively. Define candidate Cauchy functions by \begin{align} \widetilde{h}_0(w) &=2\tau_w a_2(\tau_w)-2a_3(\tau_w)+a_4(\tau_w),\label{eq:index-H0}\\ \widetilde{h}_1(w) &=i\bigl[(-\tau_w^2+\tau_w)a_2(\tau_w) +(2\tau_w-1)a_3(\tau_w)+a_5(\tau_w)\bigr]. \label{eq:index-H1} \end{align} Indeed, the lower bank uses \(\tau_w+1\); subtracting its value from the upper bank gives exactly \eqref{eq:jumps}. Conversely, subtracting these explicit jumping terms from Cauchy functions with \eqref{eq:jumps} leaves periodic remainders \(a_4,a_5\). Their definition for an actual coefficient solution is carried out on a fundamental domain in Lemma~\ref{lem:coefficients-to-section}. Let \(I_r\) denote the \(r\)-by-\(r\) identity matrix. Collect the six functions as \(\mathbf a=(a_0,a_1,a_2,a_3,a_4,a_5)^T\). The translation matrix is \(\mathsf J_{\mathrm{tr}}\). To specify the inversion matrix, define the frame matrix \(\mathsf S_{\mathrm{frm}}(\tau)\) and the matrix \(\mathsf S_{\mathrm{swap}}\) that interchanges two triples: \[ \mathsf J_{\mathrm{tr}}=\operatorname{diag}(1,1,1,-1,1,1),\qquad \mathsf S_{\mathrm{swap}}=\begin{pmatrix}0&I_3\\I_3&0\end{pmatrix}, \] \begin{equation} \mathsf S_{\mathrm{frm}}(\tau)= \begin{pmatrix} 1&\tau&\tau^2&1&0&0\\ 0&1&2\tau&0&0&0\\ 0&\tau^{-1}&1&2&0&0\\ 0&0&1&2&0&0\\ 0&0&-1-2\tau&0&-1&0\\ 0&0&\tau^2&1&0&-1 \end{pmatrix},\qquad \mathsf J_{\mathrm{inv}}(\tau)=\mathsf S_{\mathrm{frm}}(-1/\tau)^{-1}\mathsf S_{\mathrm{swap}}\mathsf S_{\mathrm{frm}}(\tau). \label{eq:J} \end{equation} The gluing laws are \begin{equation} \mathbf a(\tau+1)=\mathsf J_{\mathrm{tr}}\mathbf a(\tau),\qquad \mathbf a(-1/\tau)=\tau^{-10}\mathsf J_{\mathrm{inv}}(\tau)\mathbf a(\tau). \label{eq:automorphy} \end{equation} All matrices are holomorphic and invertible in the upper half-plane: \(\det\mathsf S_{\mathrm{frm}}=-4\) and \(\det\mathsf J_{\mathrm{inv}}=-1\). Writing \(S\tau=-1/\tau\), \(T\tau=\tau+1\), \(R_3=ST\), and \(\mathsf J_{ST}(\tau)=\mathsf J_{\mathrm{inv}}(\tau+1)\mathsf J_{\mathrm{tr}}\), direct multiplication gives \begin{equation} \mathsf J_{\mathrm{inv}}(S\tau)\mathsf J_{\mathrm{inv}}(\tau)=I_6,\qquad \mathsf J_{ST}(R_3^2\tau)\mathsf J_{ST}(R_3\tau) \mathsf J_{ST}(\tau)=I_6. \label{eq:group-relations} \end{equation} The scalar weight factors also have product \(1\). The transformations \(S,T\) generate the modular group \(\PSL=\SL/\{\pm I_2\}\), acting on \(\mathbb H\) by fractional linear transformations. The group relations say that applying \eqref{eq:automorphy} along two words representing the same transformation gives the same result. This consistency is what is meant here by a holomorphic automorphy factor. The inversion matrix \(\mathsf J_{\mathrm{inv}}(\tau)\) in \eqref{eq:J} can be recovered directly from the boundary data. The first three entries of \(\mathsf S_{\mathrm{frm}}(\tau)\mathbf a(\tau)\) are the following expressions, in which all six scalar functions are evaluated at \(\tau\): \[ a_0+\tau a_1+\tau^2a_2+a_3,\quad a_1+2\tau a_2,\quad a_1/\tau+a_2+2a_3. \] The last three are \[ a_2+2a_3,\quad -(1+2\tau)a_2-a_4,\quad \tau^2a_2+a_3-a_5. \] Substituting \eqref{eq:index-H0}--\eqref{eq:index-H1} in both outer traces pairs the two triples by inversion. More explicitly, write \(\widetilde{\mathbf h} =(\widetilde{h}_0,\widetilde{h}_1)^T\). For this check, the four expressions \(A_j(Q(z))\) are obtained from \(a_j(iz)\) by reversing their definitions, and \(b_0(z),b_1(z)\) are formed using \eqref{eq:BL}. For \(z\in z_+((0,1))\) or \(z\in z_-((0,1))\), evaluate the candidate Cauchy functions at \(\omega(z)\). Equation~\eqref{eq:automorphy} gives the first identity below on the first path and the second identity on the second path: \begin{align} z^{10}\widetilde{\mathbf h}(\omega(z)) &=\begin{pmatrix}b_0(z)-ib_1(z)\\z^{-1}(b_0(z)-ib_1(z))+i\Aplus(Q(z))\end{pmatrix} ,\nonumber\\ z^{10}\widetilde{\mathbf h}(\omega(z)) &=\begin{pmatrix}-b_0(z)-ib_1(z)\\-z^{-1}(b_0(z)+ib_1(z))+i\Aplus(Q(z))\end{pmatrix} . \label{eq:outer-check} \end{align} For these evaluations, put \(\tau=iz\). The logarithmic parameter of \(\omega(z)\) is \(-1/\tau\) on the first arc and \(-1/\tau+1\) on the second. These are algebraic row identities in \(\mathsf J_{\mathrm{inv}}\) and \(\mathsf J_{\mathrm{tr}}\). To show that every coefficient solution produces these transformation laws, we must extend its functions over a full fundamental domain. Lemma~\ref{lem:coefficients-to-section} establishes this direction. \subsection{Cusp conditions and equivalence} The end \(\Im\tau\to\infty\) is called the modular cusp. Let \(\cuspq\) be a local complex coordinate at this cusp: substitution of \(\cuspq=e^{2\pi i\tau}\) converts Laurent series in \(\cuspq\) into periodic functions of \(\tau\). The half-power \(\cuspq^{1/2}\) means \(e^{\pi i\tau}\) when pulled back to the upper half-plane. Thus the cusp corresponds to \(\cuspq=0\). It is distinct from the contour cusp \(w_c\) treated in Section~\ref{sec:regularity}. At this modular cusp, prescribe the following bounds: \begin{equation} \begin{array}{c|rrrrrr} \text{function}&a_0&a_1&a_2&a_3&a_4&a_5\\ \hline \text{lowest allowed exponent of }\cuspq &-2&-1&1&\tfrac12&-1&-1. \end{array} \label{eq:cusp-orders} \end{equation} Each function is \(\cuspq\) to the displayed exponent times a convergent power series in \(\cuspq\). In particular, \(a_4,a_5\) may each have a simple pole. Write their principal parts as \(\kappa_0\cuspq^{-1}/(2\pi i)\) and \(-\kappa_1\cuspq^{-1}/(2\pi)\), respectively. The constants \(\kappa_0,\kappa_1\) are not prescribed in this global problem. Lemma~\ref{lem:reconstruction} will identify them with the zeroth moments \(m_{0,0},m_{1,0}\) of the recovered coefficient vector. The constant terms of \(a_4,a_5\) are also unrestricted. Neither \(\lambda=1\) nor \(G_{\mathbf c}(0)=1\) has been imposed here. Here is the geometric meaning of this problem. Form the quotient of \(\mathbb H\) by \(\SL\), retaining the stabilizers, and add the cusp. In this quotient the central element \(-I_2\) is retained as a stabilizer even though it acts trivially on \(\mathbb H\); the stabilizers are larger at the two elliptic points. This is the compactified modular orbifold \(\overline{\mathcal X}\), identified with the weighted projective line \(\mathbb P(4,6)\) in \cite{CF}. The six-dimensional vectors are identified over equivalent points by \eqref{eq:automorphy}. At the cusp, divide each component by its displayed power in \eqref{eq:cusp-orders}; these quotients are the coordinates required to be holomorphic there. Explicitly, write \(\kappa_{\mathrm{cusp},j}\), \(0\leq j\leq5\), for the six exponents in \eqref{eq:cusp-orders}, and put \[ \mathsf S_{\mathrm{cusp}}(\tau) =\operatorname{diag}\bigl(e^{2\pi i\kappa_{\mathrm{cusp},j}\tau}\bigr)_{j=0}^5. \] Then \(\mathsf S_{\mathrm{cusp}}(\tau+1) =\mathsf J_{\mathrm{tr}}\mathsf S_{\mathrm{cusp}}(\tau)\). Thus \(\mathsf S_{\mathrm{cusp}}^{-1}\mathbf a\) is a single-valued vector function of \(\cuspq\), and requiring it to be holomorphic at zero defines the cusp trivialization. In particular the half-integer exponent cancels the fourth component's antiperiodicity. These rules define a rank-six holomorphic vector bundle \(\mathcal E\). For the arguments below, a global section of \(\mathcal E\) means exactly a vector of six holomorphic functions on \(\mathbb H\) satisfying \eqref{eq:automorphy} and \eqref{eq:cusp-orders}. We denote the vector space of these sections by \(H^0(\overline{\mathcal X},\mathcal E)\), or simply \(H^0(\mathcal E)\). The geometric description allows us to apply Riemann--Roch in Section~\ref{sec:index}. \subsection{From a section to the coefficient equations} \begin{lemma}\label{lem:section-to-coefficients} Taking the Laurent coefficients of the first four components defines an injective linear map \[ H^0(\overline{\mathcal X},\mathcal E) \longrightarrow\ker_{\ell^2(\mathcal I_{24})}\Mom. \] Every coefficient vector in its image is absolutely summable with weight \(r^m\) for every \(10, \ |z|>1,\ |z-i|>1\}. \] Its image under $\tau=iz$ is the fundamental domain \[ -1<\Re\tau<0,\qquad |\tau|>1,\qquad|\tau+1|>1, \] with its two halves related to the usual fundamental domain by a translation. For the following domain checks write $\sigma=\Re z$ and $t=\Im z$. On the part $\sigma>1$ the four coefficient functions already exist. On the cap $\sigma<1$, both $z$ and $z-i$ lie in the two respective halves of $\mathcal D$. Indeed, \[ \sqrt{1-\sigma^2}\sqrt{1-r^2}\ge h_\Omega(r)\). For the last inequality put \(x=\sqrt{1-r^2}\). Then \(2x-1\geq0\), and \((2x-1)^2-(1-4r^2)=4(1-x)\geq0\). This also proves \(1/z\in\mathcal W\), the domain on which \(\mathbf h_{\mathrm{par}}(1/z)\) was defined. Since $\tau=iz$ has $-1<\Re\tau<0$, the chosen logarithm of \(e^{-2\pi z}\) corresponds to $\tau+1$. Therefore set \begin{align} a_4(\tau)&=h_0(e^{2\pi i\tau}) -2(\tau+1)a_2(\tau)-2a_3(\tau),\\ a_5(\tau)&=h_1(e^{2\pi i\tau})/i +(\tau^2+\tau)a_2(\tau) +(2\tau+1)a_3(\tau). \label{eq:converse-p-fields} \end{align} \textit{The translation sides.}\quad The sides \(t=0,1\) of \(\mathcal R\) have \(\sigma>1\). There the original series converge normally. Their parity gives the translation law for the first four components. The two traces of \(h_\nu(e^{2\pi i\tau})\) differ by \eqref{eq:jumps}; subtracting the polynomial terms displayed in \eqref{eq:converse-p-fields} cancels that difference. For example, across the positive slit the logarithmic parameter changes from \(\tau\) to \(\tau+1\); \(a_2(\tau+1)=a_2(\tau)\) and \(a_3(\tau+1)=-a_3(\tau)\). The difference of the terms \(2\tau a_2-2a_3\) is \(-2a_2-4a_3=2A_-\), exactly the first jump. Subtracting the terms in \eqref{eq:index-H1} similarly gives \(2i\tau(a_2+2a_3)=-\pi^{-1}(\log s)A_-\). The remaining components \(a_4,a_5\) consequently match periodically. Lemma~\ref{lem:trace-gluing} glues the functions across these open sides, giving the full translation law. \textit{The curved sides.}\quad We specify the ordered Cauchy inputs and the recovery matrices to check these identifications without assuming any continuation law. Write \[ \mathbf h_{\mathrm{cell}}(z)=\begin{pmatrix}h_{0,\mathrm{par}}(z)\\h_{1,\mathrm{par}}(z)/i\end{pmatrix}. \] On the cap the four coefficient functions are recovered from \begin{equation} \begin{pmatrix}\mathbf h_{\mathrm{cell}}(z)\\\mathbf h_{\mathrm{cell}}(z-i)\end{pmatrix} =\mathsf S_{\mathrm{cell}}(\tau) \begin{pmatrix}a_0\\a_1\\a_2\\a_3\end{pmatrix}, \qquad \tau=iz, \label{eq:cell-recovery} \end{equation} where \[ \mathsf S_{\mathrm{cell}}(\tau)= \begin{pmatrix} 1&\tau+1&\tau^2+2\tau&1\\ \tau^{-1}&1+\tau^{-1}&\tau+1&2+\tau^{-1}\\ -1&-\tau&1-\tau^2&1\\ -(\tau+1)^{-1}&-\tau/(\tau+1)&-\tau&-(2\tau+1)/(\tau+1) \end{pmatrix}, \qquad \det\mathsf S_{\mathrm{cell}}=-4. \] The relation to the earlier paired-trace matrix is \[ \mathsf S_{\mathrm{cell}}(\tau) =\operatorname{diag}(1,-i,1,-i)\, \mathsf S_{\mathrm{pair}}(-i\tau)\, \operatorname{diag}(1,i,-1,1). \] The two diagonal factors simply implement the changes from \(\mathbf h_{\mathrm{par}}\) to \(\mathbf h_{\mathrm{cell}}\) and from \(\mathbf a_{\mathrm{ser}}\) to \((a_0,a_1,a_2,a_3)^T\). Define a six-by-six rational recovery matrix $\mathsf S_{\mathrm{rec}}^{(24)}(\tau)$ by the following recipe on three two-component inputs $\mathbf b_1,\mathbf b_2,\mathbf b_3$, where $\mathbf b_j=(b_{j,0},b_{j,1})^T$: \begin{align*} (a_0,a_1,a_2,a_3)^T &=\mathsf S_{\mathrm{cell}}(\tau)^{-1} (\mathbf b_1^T,\mathbf b_2^T)^T,\\ a_4&=-\tau^{10}b_{3,0}-2(\tau+1)a_2-2a_3,\\ a_5&=-\tau^{10}b_{3,1}+(\tau^2+\tau)a_2+(2\tau+1)a_3. \end{align*} The actual six functions on the cap are thus \[ \mathbf a(\tau)=\mathsf S_{\mathrm{rec}}^{(24)}(\tau) \begin{pmatrix}\mathbf h_{\mathrm{cell}}(z)\\\mathbf h_{\mathrm{cell}}(z-i)\\\mathbf h_{\mathrm{cell}}(1/z)\end{pmatrix}. \] For the third input, $\mathbf h_{\mathrm{par}}(1/z)=z^{-10} \mathbf h(e^{-2\pi z})$, so this expression agrees with \eqref{eq:converse-p-fields}. Consider the curved side $|z|=1$, $0<\Im z<1/2$, and put $z_1=z-i$, $z_2=1/z+i$. Its partner is $z_2$ on the other curved side. The elementary identities \[ \frac1{z_2}=\frac1{z_1}-i,\qquad e^{-2\pi/(1/z_2)}=e^{-2\pi/z} \] and the single-valuedness of $\mathbf h$ across the negative real axis give \begin{equation} \mathbf h_{\mathrm{cell}}(z_2)=\tau^{-10}\mathbf h_{\mathrm{cell}}(z_1),\qquad \mathbf h_{\mathrm{cell}}(z_2-i)=\mathbf h_{\mathrm{cell}}(1/z),\qquad \mathbf h_{\mathrm{cell}}(1/z_2)=(1+\tau)^{-10}\mathbf h_{\mathrm{cell}}(z). \label{eq:cell-cauchy-matching} \end{equation} These identities hold in a neighborhood of each open side point. For example, on that side $e^{-2\pi/z_1}$ and $e^{-2\pi/z_2}$ are the same negative real point strictly inside $\Omega$, so this matching does not cross the cut or appeal to an unknown continuation. Let $\mathsf S_{\mathrm{match}}^{(24)}(\tau)$ denote the block matrix \[ \begin{pmatrix} 0&\tau^{-10}I_2&0\\ 0&0&I_2\\ (1+\tau)^{-10}I_2&0&0 \end{pmatrix}. \] Substituting the displayed recovery recipe gives the rational identity \begin{equation} \mathsf J_{\mathrm{tr}}\mathsf S_{\mathrm{rec}}^{(24)}(-1/\tau-1) \mathsf S_{\mathrm{match}}^{(24)}(\tau) =\tau^{-10}\mathsf J_{\mathrm{inv}}(\tau)\mathsf S_{\mathrm{rec}}^{(24)}(\tau). \label{eq:cell-matrix-matching} \end{equation} All entries are specified above, so this can be checked by direct multiplication; no identities of special modular forms enter this multiplication. Together with \eqref{eq:cell-cauchy-matching}, it proves precisely the inversion law \eqref{eq:automorphy} across the paired curved sides. This verifies the gluing for the actual solution, rather than imposing that law on it. \textit{The elliptic vertices and extension to \(\mathbb H\).}\quad At \(z=e^{i\pi/6}\), all three Cauchy arguments in the recovery formula equal \(-e^{-\pi\sqrt3}\), an interior point of the negative real interval in \(\Omega\). The matrices and coordinate maps are nonsingular there. The six recovered functions therefore extend holomorphically to a full neighborhood of this vertex in the parameter plane. At \(z=1\) and \(1+i\), Proposition~\ref{prop:regularity} makes the four coefficient functions holomorphic on neighborhoods of the vertices. The outer densities near \(w_0\) are consequently holomorphic functions on each incident arc: the map \(\omega\) has nonzero derivative at \(z=1\), and all the factors in \eqref{eq:densities} are holomorphic there. The segment density is also holomorphic near \(w_0>0\), using the local square root and real logarithm in \eqref{eq:densities}. Lemma~\ref{lem:endpoint-log}, with the correction \(1/w\) holomorphic near \(w_0\), gives \[ |h_\nu(w)|\leq C\bigl(1+|\log|w-w_0||\bigr) \] in each incident sector. Since \(e^{-2\pi z}-w_0\) has a simple zero at \(z=1\), the definitions \eqref{eq:converse-p-fields} give the same logarithmic bound for \(a_4,a_5\) at the corresponding vertex. For completeness, the gluing at a vertex takes place on the upper-half-plane cover, not merely on the quotient. Take a sufficiently small disk about the elliptic fixed point. Finitely many translates of the incident cell sectors fill the punctured disk. At the point of order two, translation first joins the sectors represented by \(z=1\) and \(1+i\); inversion supplies the remaining sectors. At the point of order three use the three sectors related by the order-three transformation. Assign functions on successive sectors by the stated side laws. The open-side identities already proved glue adjacent assignments holomorphically. A complete turn composes either the order-two relation or the order-three relation in \eqref{eq:group-relations}, including the scalar factors; the product is the identity. Thus the assignment is single-valued on this punctured disk. All transition matrices and their inverses are holomorphic and bounded on a smaller disk. The sector bounds therefore give a common bound \(C(1+|\log|\tau-\tau_*||)\) in all directions. For every \(k\geq1\), the coefficient of \((\tau-\tau_*)^{-k}\) has absolute value at most \(Cr^k(1+|\log r|)\), which tends to zero. Every negative Laurent coefficient vanishes. The six functions extend holomorphically across the fixed point, and equivariance there follows by continuity. This is precisely holomorphy in the local orbifold chart. Now extend over all translates of the cell. Across an open side the assignments agree by the identities already checked; at vertices they agree by the local argument above. The relations of \(\PSL\) ensure independence of the word used to reach a translated cell. We obtain a holomorphic vector on \(\mathbb H\) satisfying \eqref{eq:automorphy}. The retained central element \(-I_2\) acts trivially, so this vector defines a section on the modular orbifold away from the cusp. \textit{The modular cusp.}\quad The first four components still have their original series for \(\Im\tau>1\), and hence the first four exponents of \eqref{eq:cusp-orders}. The periodic components \(a_4,a_5\) are single-valued holomorphic functions of \(\cuspq\) on a punctured disk. On a slit version of that disk their expressions are the Cauchy functions minus the explicit jumping terms. The Cauchy kernel area estimate in Lemma~\ref{lem:local-area} holds also on a disk containing zero; the separate correction \(1/w\) is itself area-integrable there. The subtracted terms are bounded by constants times \(|w|\,|\log w|^2+|w|^{1/2}(1+|\log w|)\). Thus \(a_4,a_5\), as functions of \(\cuspq\), are area-integrable. Lemma~\ref{lem:area-removal} leaves at most a simple pole in each. We compute those poles without any unproved boundary estimate at zero. Split the measure in \eqref{eq:Cauchy} into its arc and segment parts, and take \(w=-r<0\), \(r\downarrow0\). The arc stays a positive distance from zero, so multiplying its Cauchy integral by \(w\) makes it tend to zero. On the segment, with variable \(s>0\), \[ \left|\frac{w}{s-w}\right|=\frac{r}{s+r}\leq1, \qquad \frac{w}{s-w}\longrightarrow0 . \] Finite total variation and the absence of an atom at zero give the same conclusion by dominated convergence. The explicit correction contributes exactly \(m_{\nu,0}/(2\pi i)\) to \(\lim_{w\to0}w h_\nu(w)\). The jumping terms contribute zero to that limit. Hence the principal parts of \(a_4,a_5\) are, respectively, \[ \frac{m_{0,0}}{2\pi i}\cuspq^{-1}, \qquad -\frac{m_{1,0}}{2\pi}\cuspq^{-1}. \] No restriction is imposed on their constant terms. These are exactly the last two conditions in \eqref{eq:cusp-orders}, so the section extends across the cusp in the prescribed frame and recovers the original coefficients. \end{proof} \begin{proposition}[Boundary--bundle correspondence]\label{prop:equivalence} The coefficient map is an isomorphism \[ H^0(\overline{\mathcal X},\mathcal E) \simeq\ker_{\ell^2(\mathcal I_{24})}\Mom. \] For every vector in this kernel, the infinite coefficient sequences are absolutely summable with weight \(r^m\), for each \(11\) is fixed and \(J\in\mathbb N\). The orthogonal projection \(\mathsf P_J:\ell^2(\mathcal I_{24})\to\ell^2(\mathcal I_{24})\) is defined to be the identity on the five entries with nonpositive exponent and to act on each infinite sequence by setting its entries with \(m>J\) to zero. Use the usual coefficient inner products on \(\ell^2(\mathcal I_{24})\), on the moment space \(\ell^2(\mathcal J_{24})\), and on \(\mathbb C\). A superscript \(*\) denotes the adjoint with respect to these inner products. Define \begin{equation} \begin{aligned} \mathsf L&=(\Id_{\mathcal I_{24}}-\mathsf K)^* (\Id_{\mathcal I_{24}}-\mathsf K)+\Mom^*\Mom,\\ \mathsf N&=\mathsf L+\lambda^*\lambda. \end{aligned} \label{eq:N} \end{equation} Both are bounded positive self-adjoint operators. They are the identity plus compact operators, and \[ \ker\mathsf L=\ker\Mom, \] because \(\langle\mathsf L\mathbf c,\mathbf c\rangle =\|(\Id_{\mathcal I_{24}}-\mathsf K)\mathbf c\|^2+\|\Mom \mathbf c\|^2\). \begin{theorem}[Bounded inverse]\label{thm:inverse} There is a constant \(c_{\mathrm{coer},24}>0\) such that, for every \(\mathbf c\in\ell^2(\mathcal I_{24})\), \begin{equation} \begin{aligned} \langle\mathsf N\mathbf c,\mathbf c\rangle &=\|(\Id_{\mathcal I_{24}}-\mathsf K)\mathbf c\|_2^2 +\|\Mom\mathbf c\|_2^2+|\lambda(\mathbf c)|^2\\ &\geq c_{\mathrm{coer},24}\|\mathbf c\|_2^2. \end{aligned} \label{eq:coercivity} \end{equation} Consequently \(\mathsf N\) is boundedly invertible and \begin{equation} \mathbf c_*=\mathsf N^{-1}\lambda^*(1). \label{eq:inverse-solution} \end{equation} \end{theorem} \begin{proof} If the inequality failed, there would be unit vectors \(\mathbf c_j\) with \[ (\Id_{\mathcal I_{24}}-\mathsf K)\mathbf c_j\to0,\qquad \Mom \mathbf c_j\to0,\qquad \lambda(\mathbf c_j)\to0. \] Compactness of \(\mathsf K\) gives a convergent subsequence of \(\mathsf K\mathbf c_j\); the same subsequence of \(\mathbf c_j\) converges to a unit vector \(\mathbf c\). Then \(\Mom \mathbf c=0\) and \(\lambda(\mathbf c)=0\), contradicting Proposition~\ref{prop:vanishing}. Coercivity gives closed range and zero kernel. Self-adjointness then gives dense range, hence surjectivity. Let \(\mathbf b\ne0\) be a vector in \(\ker\Mom\). For \(\mathbf c=\mathsf N^{-1}\lambda^*(1)\), pair the equation with \(\mathbf b\). Since \(\lambda(\mathbf b)\ne0\) and \(\mathsf L\mathbf b=0\), this gives \(\lambda(\mathbf c)=1\). The equation becomes \(\mathsf L\mathbf c=0\). Thus \(\mathbf c\) is the normalized coefficient solution. \end{proof} This also gives convergence of the exact Galerkin approximations. On \(\mathsf P_J\ell^2(\mathcal I_{24})\) solve \[ \mathsf P_J\mathsf N \mathsf P_J \mathbf c_J=\mathsf P_J\lambda^*(1). \] Every compression is coercive with the same constant \(c_{\mathrm{coer},24}\). Galerkin orthogonality and \eqref{eq:coercivity} give \[ \|\mathbf c_J-\mathbf c_*\|_2\leq \frac{\|\mathsf N\|}{c_{\mathrm{coer},24}}\|(\Id_{\mathcal I_{24}}-\mathsf P_J)\mathbf c_*\|_2 \longrightarrow0. \] The right side has a geometric tail by Theorem~\ref{thm:main}. This is a convergence statement for the positive equation \eqref{eq:N}; it does not assert stability of arbitrary finite truncations of the original compact moment map \(\Mom\). The proof establishes \(c_{\mathrm{coer},24}>0\) without supplying a numerical value. The compressed matrix still contains integrals and infinite inner products, through \(\mathsf K^*\mathsf K\) and \(\Mom^*\Mom\). A certified numerical implementation would additionally require error bounds for their evaluation, a computable coercivity bound, and control of the resulting perturbation of the finite equations. No such implementation or numerical efficiency claim is needed for the existence theorem. \section{Comparison with the known function in dimension 24}\label{sec:comparison} Existence and uniqueness in the coefficient space have now been proved. We next identify the answer. This comparison is not used in either dimension's existence or uniqueness proof. \subsection{Coefficient identification} Use \(\cuspq=e^{2\pi i\tau}\), and normalize \[ E_2=1-24\sum_{n\geq1}\sigma_1(n)\cuspq^n,\quad E_4=1+240\sum_{n\geq1}\sigma_3(n)\cuspq^n,\quad E_6=1-504\sum_{n\geq1}\sigma_5(n)\cuspq^n, \] where \(\sigma_j(n)=\sum_{\ell\mid n}\ell^j\). Here \(\Delta_{\rm mod}=(E_4^3-E_6^2)/1728\). For the comparison only, set \begin{align*} r_0&=-49E_4^3+25E_6^2,& r_1&=48E_6E_4^2,& r_2&=25E_4^4-49E_4E_6^2,\\ \varphi_{24,2}&=\frac{r_2+r_1E_2+r_0E_2^2}{\Delta_{\rm mod}^2},& \varphi_{24,1}&=\frac{-6r_1-12E_2r_0}{\Delta_{\rm mod}^2},& \varphi_{24,0}&=\frac{-36r_0}{\Delta_{\rm mod}^2}. \end{align*} Let \[ \theta_2(\tau)=\sum_{n\in\mathbb Z}e^{\pi i(n+1/2)^2\tau}, \qquad \theta_4(\tau)=\sum_{n\in\mathbb Z}(-1)^ne^{\pi in^2\tau}. \] Writing \(x=\theta_4^4,\ y=\theta_2^4\), define \[ \psi_{24,I}=\frac{7x^5y^2+7x^6y+2x^7}{\Delta_{\rm mod}^2},\qquad \psi_{24,S}=-\frac{7y^5x^2+7y^6x+2y^7}{\Delta_{\rm mod}^2}. \] These are the ingredients of \cite[Sections 2--4]{CKMRV24}: \(\varphi_{24,2}\) is a weakly holomorphic quasimodular form of weight \(-8\) and depth \(2\), and \(\psi_{24,I}\) has weight \(-10\) for \(\Gamma(2)\). Let \(f_{\rm known}\) be the normalized magic function constructed in \cite{CKMRV24}, and define \(\Phi_{\rm known}:[0,\infty)\to\mathbb R\) by \(f_{\rm known}(\mathbf y)=\Phi_{\rm known}(|\mathbf y|^2)\). For \(u>4\), it is given by \begin{equation} \Phi_{\rm known}(u)=P(u)\int_0^\infty \left(\frac{\pi}{K_{24}^{\varphi}}t^{10}\varphi_{24,2}(i/t) -\frac1{K_{24}^{\psi}\pi}\psi_{24,I}(it)\right)e^{-\pi ut}\,dt, \label{eq:known-integral} \end{equation} Here \(K_{24}^{\varphi}=28304640\) and \(K_{24}^{\psi}=65520\). The profile extends to all \(u\geq0\). The required transformation identities are \begin{align} t^{10}\varphi_{24,2}(i/t) &=t^2\varphi_{24,2}(it)+\frac{t}{\pi}\varphi_{24,1}(it) -\frac1{\pi^2}\varphi_{24,0}(it), \nonumber\\ \psi_{24,I}(it)&=-t^{10}\psi_{24,S}(i/t),& \psi_{24,S}(\tau)&=\psi_{24,I}(\tau)-\psi_{24,I}(\tau+1). \label{eq:known-transformations} \end{align} Here is an explicit translation into our coefficients. Use the cusp coordinate \(\mathfrak q=e^{2\pi i\tau}\), with \(\mathfrak q^{1/2}=e^{\pi i\tau}\). Define the scalar coefficients by \begin{align*} \varphi_{24,j}(\tau)&=\sum_m\varphi_{24,j,m}\mathfrak q^{m/2} &&(j=0,1,2),\\ \psi_{24,I}(\tau)&=\sum_m\psi_{24,I,m}\mathfrak q^{m/2},& \psi_{24,S}(\tau)&=\sum_m\psi_{24,S,m}\mathfrak q^{m/2}. \end{align*} The indices \(m\) are integers and only finitely many negative powers occur. For example, \(\varphi_{24,2,m}=[\mathfrak q^{m/2}]\varphi_{24,2}\) denotes the scalar coefficient of \(\mathfrak q^{m/2}\) in this expansion. The brackets denote coefficient extraction. The relation to our generating-series variable is \(q=e^\pi\mathfrak q^{1/2}\). The second subscript \(j\) in \(\varphi_{24,j}\) is chosen so that its weight is \(2j-12\), matching the three polynomial degrees in the large-parameter integrals. Split \eqref{eq:known-integral} at \(t=1\), and use \eqref{eq:known-transformations} on the appropriate halves. The large-parameter coefficients before damping are \begin{align} \gamma_{24,0,m}&=-\frac{\varphi_{24,0,m}+432\psi_{24,I,m}}{K_{24}^{\varphi}\pi},\nonumber\\ \gamma_{24,1,m}&=\frac{\varphi_{24,1,m}}{K_{24}^{\varphi}},\nonumber\\ \gamma_{24,2,m}&=\frac{\pi \varphi_{24,2,m}}{K_{24}^{\varphi}}, \label{eq:known-c} \end{align} and the small-parameter coefficient is \[ \beta_{24,m}=\frac{\pi \varphi_{24,2,m}}{K_{24}^{\varphi}} +\frac{\psi_{24,S,m}}{K_{24}^{\psi}\pi}. \] Each of \(\varphi_{24,0},\varphi_{24,1},\varphi_{24,2}\) has only even powers of \(\cuspq^{1/2}\), and \(\psi_{24,S,m}=(1-(-1)^m)\psi_{24,I,m}\). Thus \(\beta_{24,m}=\gamma_{24,2,m}\) for even \(m\), and \(\beta_{24,m}=-2\gamma_{24,0,m}\) for odd \(m\). These are exactly the parity relations in \eqref{eq:ansatz}. Because the elementary profiles \(U_{m,k}\) and \(V_m\) include the factor \(e^{\pi m}\), the corresponding sequence coefficients in \eqref{eq:ansatz} are \[ c_{j,m}=e^{-\pi m}\gamma_{24,j,m}\quad(m\ {\rm even}),\qquad c_{3,m}=e^{-\pi m}\gamma_{24,0,m}\quad(m\ {\rm odd}). \] In particular the two functions from the splitting in Section~\ref{sec:vanishing} satisfy \[ a_2^+=-\frac{\pi}{K_{24}^{\varphi}}\varphi_{24,2},\qquad a_2^-=-\frac1{2K_{24}^{\psi}\pi}\psi_{24,S}. \] The quasimodular and level-two structures thus agree with the structures derived from the boundary equations. The five coefficients of the correction functions are \(c_{j,m}=e^{-\pi m}\gamma_{24,j,m}\) at \((j,m)=(0,-4),(0,-2),(0,0),(1,-2),(1,0)\). There are no other nonpositive modes. In particular the resulting finite part is \begin{equation} 4R_{0,1}-\frac{R_{4,0}}{16380\pi} -\frac{14347}{1365\pi}R_{0,0} +\frac1{39}R_{2,1}-\frac{292}{4095\pi}R_{2,0}. \label{eq:finite-known} \end{equation} These identities follow by multiplication of the displayed series; they also check the normalization of the coefficient coordinates. Convergence of these expansions for \(|\mathfrak q^{1/2}|<1\), with only the stated poles at \(0\), gives weighted absolute summability after the damping factor. The split integral first identifies the two profiles for \(u>4\). Here is the analytic domain needed to extend this identity. Subtract the finitely many nonpositive exponential modes from the large-\(t\) integrand and integrate them explicitly, giving the entire correction functions in \eqref{eq:finite-known}. The remaining large-\(t\) integrand decays at least as a polynomial times \(e^{-\pi t}\), and the small-\(t\) integrand decays exponentially in \(1/t\). The resulting integrals converge normally for complex \(u\) on compact subsets of \(\Re u>-1\). They give the analytic continuation used in \cite[Sections 2--4]{CKMRV24}. Our coefficient profile is holomorphic on this same half-plane by the normal-convergence estimates in Lemma~\ref{lem:Schwartz}; its possible negative integer poles lie outside it. The identity theorem gives equality throughout \(\Re u>-1\), and in particular at all nonnegative real \(u\). The known Fourier zeros and normalization now show that the coefficient vector solves \eqref{eq:system}. Theorem~\ref{thm:main} identifies it with \(\mathbf c_*\). Consequently the sign inequalities proved in \cite{CKMRV24} hold for \(f_{\mathbf c_*}\). In this sense the coefficient construction recovers the Leech lattice magic function. \subsection{The alternative uniqueness argument from interpolation} The interpolation theorem of \cite[Theorems 1.7 and 1.9]{CKMRVinterp} states that a radial Schwartz function on \(\mathbb R^{24}\) is determined by the values and radial derivatives of itself and its Fourier transform at \(\sqrt{2n}\), \(n\geq2\). For our normalized function, all these data vanish except the radial derivative \[ \left.\frac{d}{dr}\Phi_{\mathbf c_*}(r^2)\right|_{r=2} =4\Phi_{\mathbf c_*}'(4)=-\frac1{16380}. \] In the interpolation basis of that paper this says \[ f_{\mathbf c_*}=-\frac1{16380}b_2, \] where \(b_2\) has radial derivative \(1\) at \(2\) and all other interpolation data zero. It follows at once that the function is unique in the full radial Schwartz class with these data. Injectivity in Lemma~\ref{lem:Schwartz} then gives coefficient uniqueness as well. This is an alternative argument, not a premise of our proof. Our independent uniqueness statement is within the coefficient class \eqref{eq:ansatz}; the assertion about all radial Schwartz functions uses the interpolation theorem. \section{The construction in dimension 8}\label{sec:eight} \label{sec:dimension} We now prove the analogous theorem for \(E_8\). The first nonzero squared length is \(2\), so the Fourier equations start one node earlier. This removes two correction functions and forces the constant moments to vanish. Gaussian inversion changes the scalar power from \(10\) to \(2\). We give the resulting system explicitly, check the continuation problem and its index, and prove uniqueness. None of these steps uses the comparison with the known function in Section~\ref{sec:eight-comparison}. \subsection{The coefficient system and its theorem} Keep \(P,U_{m,k},R_{\ell,k}\) as defined in \eqref{eq:U} and \eqref{eq:Hfinite}, and define \begin{equation} V_m^{(8)}(u)=e^{\pi m}P(u)\int_0^1 t^2e^{-\pi(m/t+ut)}\,dt, \qquad u\geq0,\quad m\in\mathbb N. \label{eq:eight-V} \end{equation} The power is \(d/2-2=2\): Gaussian inversion contributes \(t^{-d/2}\), and the substitution \(t\mapsto1/t\) contributes its Jacobian. The large-parameter integrals \(U_{m,k}\) do not change. Define \[ \mathcal I_8=\{(0,-2),(0,0),(1,0)\}\cup\mathcal I_+. \] An eight-dimensional coefficient vector \(\mathbf c=(c_{j,m})_{(j,m)\in\mathcal I_8}\) consists of the three numbers \(c_{0,-2},c_{0,0},c_{1,0}\), three sequences \((c_{k,m})_{m\in2\mathbb N}\), \(k=0,1,2\), and one sequence \((c_{3,m})_{m\in2\mathbb N-1}\). For \(p=1,2\), define \begin{equation} \|\mathbf c\|_{p,8}^p= |c_{0,-2}|^p+|c_{0,0}|^p+|c_{1,0}|^p +\sum_{m\in2\mathbb N}\sum_{k=0}^2|c_{k,m}|^p +\sum_{m\in2\mathbb N-1}|c_{3,m}|^p. \label{eq:eight-norm} \end{equation} Write \(\ell^p(\mathcal I_8)\) for the space of these families with finite norm. Thus \(\ell^p(\mathcal I_8)=\mathbb C^3\oplus\ell^p(2\mathbb N)^3 \oplus\ell^p(2\mathbb N-1)\). These are new coefficient vectors; they are not the dimension-24 solutions with two entries removed. For \(\mathbf c\in\ell^2(\mathcal I_8)\), set \begin{align} \Phi^{(8)}_{\mathbf c}(u)={}& c_{1,0}R_{0,1}(u)+c_{0,0}R_{0,0}(u) +e^{-2\pi}c_{0,-2}R_{2,0}(u)\nonumber\\ &+\sum_{m\in2\mathbb N-1}c_{3,m} \bigl(U_{m,0}(u)-2V_m^{(8)}(u)\bigr)\nonumber\\ &+\sum_{m\in2\mathbb N} \bigl(c_{0,m}U_{m,0}(u)+c_{1,m}U_{m,1}(u) +c_{2,m}(U_{m,2}(u)+V_m^{(8)}(u))\bigr). \label{eq:eight-family} \end{align} Define \(f^{(8)}_{\mathbf c}(\mathbf y)=\Phi^{(8)}_{\mathbf c}(|\mathbf y|^2)\) for \(\mathbf y\in\mathbb R^8\), and define \(G^{(8)}_{\mathbf c}\) on \([0,\infty)\) by \(\widehat f^{(8)}_{\mathbf c}(\boldsymbol{\xi})=G^{(8)}_{\mathbf c}(|\boldsymbol{\xi}|^2)\). The Fourier transform here is taken in \(\mathbb R^8\). Finally put \(\lambda_8(\mathbf c)=c_{1,0}/4\). \begin{theorem}[Eight-dimensional coefficient construction] \label{thm:eight} The countable system of linear equations \begin{equation} G^{(8)}_{\mathbf c}(2n)=(G^{(8)}_{\mathbf c})'(2n)=0 \quad(n\geq1),\qquad \lambda_8(\mathbf c)=1 \label{eq:eight-system} \end{equation} has exactly one solution \(\mathbf c_{*,8}\in\ell^2(\mathcal I_8)\). Its entries are real, and for every \(10\), Gaussian inversion in \(\mathbb R^8\) is \[ \widehat{\bigl(\mathbf y\mapsto e^{-\pi z|\mathbf y|^2}\bigr)}(\boldsymbol{\xi}) =z^{-4}e^{-\pi|\boldsymbol{\xi}|^2/z}. \] Consequently define \(\rho_{0,\Gamma}^{(8)},\rho_{1,\Gamma}^{(8)}\) by the four formulas in \eqref{eq:densities}, replacing the powers \(z_\pm(t)^{-10},z_\pm(t)^{-11}\) by \(z_\pm(t)^{-2},z_\pm(t)^{-3}\), respectively. The segment densities are unchanged: \[ \rho_{0,I}^{(8)}(s)=2A_-(e^\pi\sqrt s),\qquad \rho_{1,I}^{(8)}(s)=-\pi^{-1}(\log s)\,A_-(e^\pi\sqrt s) \quad(01\) and \(C_8<\infty\), independent of the solution, such that the four functions continue to \(0<|q|0. \] Thus \(\mathsf N_8\) has a bounded inverse and \(\mathbf c_{*,8}=\mathsf N_8^{-1}\lambda_8^*(1)\). The exact finite-dimensional positive compressions converge by the same Galerkin argument, subject to the distinction between exact entries and certified numerical evaluation made in Section~\ref{sec:operator}. This completes the coefficient construction before any comparison with Viazovska's function. \subsection{Identification with Viazovska's function} \label{sec:eight-comparison} We now identify the answer, using \cite[Sections 4--5]{V}. This comparison is not part of the preceding existence or uniqueness proof. Use the Eisenstein series, discriminant, and theta functions from Section~\ref{sec:comparison}, and also define \(\theta_3(\tau)=\sum_{n\in\mathbb Z}e^{\pi in^2\tau}\). Set \[ \varphi_{8,0}=\frac{E_4^2}{\Delta_{\rm mod}},\qquad \varphi_{8,1}=\frac{E_4^2E_2-E_4E_6}{\Delta_{\rm mod}},\qquad \varphi_{8,2}=\frac{(E_4E_2-E_6)^2}{\Delta_{\rm mod}}. \] \begin{align*} \psi_{8,I}&=128\left( \frac{\theta_3^4+\theta_4^4}{\theta_2^8} +\frac{\theta_4^4-\theta_2^4}{\theta_3^8}\right),\\ \psi_{8,S}&=-128\left( \frac{\theta_3^4+\theta_2^4}{\theta_4^8} +\frac{\theta_2^4-\theta_4^4}{\theta_3^8}\right). \end{align*} All functions on the right are evaluated at \(\tau\in\mathbb H\). The second subscript \(j=0,1,2\) in \(\varphi_{8,j}\) has the same role as in dimension \(24\): the weight is \(2j-d/2\), now \(-4,-2,0\). The first subscript specifies the dimension. Let \(\Phi^{(8)}_{\rm known}\) be the profile of Viazovska's normalized function. For \(u>2\), its integral formula is \begin{equation} \Phi^{(8)}_{\rm known}(u)=P(u)\int_0^\infty \left(-\frac\pi{2160}t^2\varphi_{8,2}(i/t) -\frac1{60\pi}\psi_{8,I}(it)\right)e^{-\pi ut}\,dt. \label{eq:eight-known} \end{equation} The transformation identities needed to split this integral are \begin{align} t^2\varphi_{8,2}(i/t)&=t^2\varphi_{8,2}(it) -\frac{12t}{\pi}\varphi_{8,1}(it) +\frac{36}{\pi^2}\varphi_{8,0}(it),\nonumber\\ \psi_{8,I}(it)&=-t^2\psi_{8,S}(i/t),\nonumber\\ \psi_{8,S}(\tau)&=\psi_{8,I}(\tau)-\psi_{8,I}(\tau+1). \label{eq:eight-known-laws} \end{align} Define the scalar coefficients of the cusp expansions by \begin{align*} \varphi_{8,j}(\tau)&=\sum_m\varphi_{8,j,m}\mathfrak q^{m/2} &&(j=0,1,2),\\ \psi_{8,I}(\tau)&=\sum_m\psi_{8,I,m}\mathfrak q^{m/2},& \psi_{8,S}(\tau)&=\sum_m\psi_{8,S,m}\mathfrak q^{m/2}. \end{align*} Here again \(\mathfrak q^{1/2}=e^{\pi i\tau}\), and the coefficients are numbers, defined by coefficient extraction. Splitting \eqref{eq:eight-known} at \(t=1\) and applying \eqref{eq:eight-known-laws} gives the undamped large-parameter coefficients \begin{align} \gamma_{8,0,m}&=-\frac{\varphi_{8,0,m}+\psi_{8,I,m}}{60\pi},\nonumber\\ \gamma_{8,1,m}&=\frac{\varphi_{8,1,m}}{180},\nonumber\\ \gamma_{8,2,m}&=-\frac{\pi \varphi_{8,2,m}}{2160}, \label{eq:eight-known-coefficients} \end{align} and the small-parameter coefficients \[ \beta_{8,m}=-\frac{\pi \varphi_{8,2,m}}{2160} +\frac{\psi_{8,S,m}}{60\pi}. \] All three \(\varphi_{8,j}\) have only even powers, and \(\psi_{8,S,m}=(1-(-1)^m)\psi_{8,I,m}\). Hence \(\beta_{8,m}=\gamma_{8,2,m}\) for even \(m\), and \(\beta_{8,m}=-2\gamma_{8,0,m}\) for odd \(m\). The coefficients with positive exponent \(m\) in \eqref{eq:eight-family} are \[ c_{k,m}=e^{-\pi m}\gamma_{8,k,m}\quad(m\in2\mathbb N), \qquad c_{3,m}=e^{-\pi m}\gamma_{8,0,m}\quad(m\in2\mathbb N-1). \] The permitted coefficients with exponent \(m\leq0\) are obtained by the same rule \(c_{k,m}=e^{-\pi m}\gamma_{8,k,m}\). For clarity, the coefficients at powers \(\mathfrak q^{-1},\mathfrak q^0\) of \((\varphi_{8,2},\varphi_{8,1},\varphi_{8,0}, \psi_{8,I})\) are respectively \[ (0,0,1,1),\qquad(0,720,504,144). \] There are no other nonpositive terms. Thus the correction part is exactly \begin{equation} 4R_{0,1}-\frac{R_{2,0}}{30\pi} -\frac{54}{5\pi}R_{0,0}. \label{eq:eight-known-finite} \end{equation} In particular its normalization is one. These Laurent series, viewed in the variable \(\mathfrak q^{1/2}\), converge for \(|\mathfrak q^{1/2}|<1\), apart from the stated poles at zero. Cauchy's estimates give weighted absolute summability after the factor \(e^{-\pi m}\). The split integral gives equality of the profiles for \(u>2\). Subtracting its nonpositive large-\(t\) modes gives the entire correction functions in \eqref{eq:eight-known-finite}. The remaining large-\(t\) integrand decays at least as a polynomial times \(e^{-\pi t}\), and the small-\(t\) part decays exponentially in \(1/t\). As in the preceding comparison, these expressions define holomorphic profiles on the common connected domain \(\Re u>-1\); this is the continuation of the original contour formula in \cite[Sections 4--5]{V}. The identity theorem therefore gives equality for every nonnegative real \(u\). The known Fourier zeros and normalization make the coefficient vector a solution of \eqref{eq:eight-system}, and Theorem~\ref{thm:eight} identifies it with \(\mathbf c_{*,8}\). The signs proved in \cite[Theorem 4]{V} therefore hold for our function. Fourier interpolation gives the parallel uniqueness statement in the full radial Schwartz class. By \cite[Theorems 1.7 and 1.9]{CKMRVinterp}, the data at \(\sqrt{2n}\), \(n\geq1\), determine such a function in \(\mathbb R^8\). All our interpolation data are zero except \[ \left.\frac{d}{dr}\Phi^{(8)}_{\mathbf c_{*,8}}(r^2) \right|_{r=\sqrt2}=-\frac1{30\sqrt2}. \] If \(b_1^{\rm int}\) denotes the interpolation basis function whose radial derivative at \(\sqrt2\) is one and whose other data vanish, then \(f^{(8)}_{\mathbf c_{*,8}}=-(30\sqrt2)^{-1}b_1^{\rm int}\). The superscript marks an interpolation basis function. This identification is an additional consequence, not an input to the construction. \section{The remaining sign problem}\label{sec:signs} Theorems~\ref{thm:main} and \ref{thm:eight} solve the coefficient systems: they produce real radial Schwartz functions with the required zeros, normalization, and first derivative. To complete an independent Cohn--Elkies proof, one must still establish \[ \Phi^{(8)}_{\mathbf c_{*,8}}(u)\leq0\ (u\geq2),\qquad G^{(8)}_{\mathbf c_{*,8}}(v)\geq0\ (v\geq0), \] and \[ \Phi_{\mathbf c_*}(u)\leq0\ (u\geq4),\qquad G_{\mathbf c_*}(v)\geq0\ (v\geq0). \] Prescribing values and first derivatives at a discrete set does not establish these inequalities on the intervals between nodes. Nor does an index or a uniqueness argument establish a sign. Our comparisons prove that the inequalities hold by transferring the earlier sign theorems. Without that comparison, the global sign proof in both dimensions remains unfinished. Thus we have an independent construction of the functions, not yet a complete independent proof of the sphere-packing bounds. It is useful to distinguish this situation from the planar paper, which proves its signs within the coefficient construction \cite[Section 4 and Appendices A--B]{OpenAI}. Its finite coefficient approximations come with rigorous bounds for the error in each \(\ell^1\) coefficient list. On bounded intervals, the exact prescribed zeros are factored out. Near a zero, the lower Taylor terms of the approximation error are subtracted before division by the vanishing factor, so the error bound does not become singular. Polynomial approximations in the Bernstein basis then certify signs on entire intervals through positive Bernstein coefficients, with rigorous interval enclosures and quadrature remainder bounds. The unbounded region is controlled separately by an explicit barrier built from the trigonometric product, together with second-derivative and tail estimates. These analytic estimates are what let finitely many certified computations prove signs for the infinite coefficient series on the entire required half-lines. They are not a numerical sampling argument. Adapting that program here would require effective coefficient error bounds and sign margins suited to the dimension-eight and dimension-24 families. Our bounded-inverse theorems provide convergence, but do not supply those quantitative certificates. \appendix \section{Why these elementary functions?}\label{app:motivation} The factor \(P\) builds in the desired zeros of the physical profile. It does not determine the remaining factors in \(U_{m,k}\) and \(V_m\), nor does it explain their parity restrictions. This appendix motivates those choices by Gaussian inversion and an explicit cancellation in the Fourier samples. The calculation applies to both \(d=8\) and \(d=24\). It uses no modular form and does not assume that a nonzero coefficient solution exists. \subsection{Gaussian inversion and the two integration ranges} For a radial profile \(h\) whose associated function is Schwartz, write \(\mathcal F_d h\) for its radial Fourier profile: \[ \widehat{(\mathbf y\mapsto h(|\mathbf y|^2))}(\boldsymbol{\xi}) =(\mathcal F_d h)(|\boldsymbol{\xi}|^2). \] This is the Fourier transform in \(\mathbb R^d\), expressed in one-variable profiles; it is not the one-dimensional Fourier transform of \(h\). For \(m\geq1\), start with \[ g_m(u)=e^{\pi m}\int_1^\infty e^{-\pi mt}e^{-\pi tu}\,dt. \] Gaussian inversion and the substitution \(t=1/s\) give \begin{align} (\mathcal F_d g_m)(v) &=e^{\pi m}\int_1^\infty t^{-d/2}e^{-\pi(mt+v/t)}\,dt \nonumber\\ &=e^{\pi m}\int_0^1 s^{d/2-2}e^{-\pi(m/s+vs)}\,ds . \label{eq:app-reciprocal} \end{align} Consequently \[ U_{m,0}=P g_m,\qquad V_m^{(d)}=P\,\mathcal F_d g_m, \] where \(V_m^{(24)}=V_m\) and \(V_m^{(8)}\) is \eqref{eq:eight-V}. The power \(d/2-2\) is forced by Gaussian inversion and the Jacobian. The split at \(1\) is natural because \(1\) is fixed by inversion of the Gaussian parameter. Multiplication by \(P\) does not commute with \(\mathcal F_d\), so these identities alone do not determine the Fourier samples of \(U_{m,0}\) or \(V_m^{(d)}\). That is the purpose of the next calculation. The factor \(e^{\pi m}\) normalizes the exponential mode at the splitting point: \[ e^{\pi m}e^{-\pi mt}=e^{-\pi m(t-1)}. \] It therefore makes the coefficient series converge in the variable \(q=Q(t)=e^{-\pi(t-1)}\) on the unit disk. For each fixed \(m\), it is a scalar normalization of the profile; the coefficient norm is then prescribed in these coordinates. Finally, polynomial weights in \(t\) give elementary rational factors: \begin{equation} U_{m,k}(u)=P(u)e^{-\pi u} \sum_{j=0}^k\frac{k!}{(k-j)![\pi(m+u)]^{j+1}}. \label{eq:app-rational} \end{equation} Thus \(k=0,1,2\) permits successively higher principal parts at the negative modes while preserving all the physical zeros. \subsection{The parity restrictions and the coupled terms} Let \(p\) be a polynomial with real coefficients and define \[ U_m[p](u)=e^{\pi m}P(u) \int_1^\infty p(t)e^{-\pi(m+u)t}\,dt. \] For \(p(t)=t^k\) this is \(U_{m,k}\). Put \(\sigma_m=(-1)^m\) and define the polynomial \begin{equation} (\delta_m p)(t)=2p(t)-\sigma_m\bigl(p(t+i)+p(t-i)\bigr). \label{eq:app-difference} \end{equation} The sign \(\sigma_m\) comes from shifting the exponential mode by \(i\) or \(-i\). To see this precisely, use \[ P(u)e^{-\pi tu} =\frac14\bigl(2e^{-\pi tu} -e^{-\pi(t-i)u}-e^{-\pi(t+i)u}\bigr). \] Hold \(v\geq0\) fixed, apply Gaussian inversion, and shift the two displaced horizontal paths back to the positive real axis. For \(m\geq1\), the integrands decay exponentially at the right ends, so the connecting integrals there tend to zero. Define the remaining integral along the straight path from \(1\) to \(1+i\) by \[ J_m[p](v)=e^{\pi m}\int_1^{1+i} p(z-i)z^{-d/2}e^{-\pi(mz+v/z)}\,dz. \] The lower path contributes its complex conjugate. The result is \begin{equation} \begin{split} (\mathcal F_d U_m[p])(v) ={}&\frac{\sigma_m}{2}\Re J_m[p](v)\\ &+\frac{e^{\pi m}}4\int_1^\infty (\delta_m p)(t)t^{-d/2}e^{-\pi(mt+v/t)}\,dt. \end{split} \label{eq:app-U-transform} \end{equation} The notation \(J_m[1]\) means that the polynomial is the constant \(1\), not the monomial of degree one. For \(p(t)=t^k\), this path integral is \(J_{m,k}\) from the sample calculation, with the exponent appropriate to \(d\). There is a companion identity for the reciprocal family. Let \(W_m(v)=e^{-\pi v}/(2\pi(m+v))\), as in the sample calculation. Then \begin{equation} \begin{split} (\mathcal F_d V_m^{(d)})(v) ={}&W_m(v) +\frac{\sigma_m}{2}\Re\bigl(e^{-\pi iv}J_m[1](v)\bigr)\\ &-\frac{\sigma_m}{2}\cos(\pi v)(\mathcal F_d g_m)(v). \end{split} \label{eq:app-V-transform} \end{equation} For completeness, the unshifted Gaussian term in this calculation is \[ \frac{e^{\pi m}}2\int_0^1 t^{-2}e^{-\pi(m+v)/t}\,dt=W_m(v). \] In the other two terms, first substitute \(s=1/t\). The transformed Gaussian parameters involve \(s+i\) and \(s-i\); the identity \(s/(1+is)=-i+1/(s-i)\) and its conjugate separate the factors \(e^{\pi iv}\) and \(e^{-\pi iv}\). Shifting the resulting paths back to the real axis gives the last two terms of \eqref{eq:app-V-transform}. The constant phase \(i^{-d/2}\) equals \(1\) in both dimensions under consideration. All these identities can be differentiated in \(v\) on compact real intervals by dominated convergence. Suppose now that \(\delta_m p\) is a constant \(b\). For the combination \[ U_m[p]+\frac{b}{2\sigma_m}V_m^{(d)}, \] the sum of the unbounded real-path terms in \eqref{eq:app-U-transform}--\eqref{eq:app-V-transform} is \[ \frac b4(1-\cos(\pi v))(\mathcal F_d g_m)(v) =\frac b2 P(v)(\mathcal F_d g_m)(v). \] This has a double zero at every \(v=2n\), including \(n=0\). Its contribution to both Fourier sample equations is therefore zero. Only the fixed finite path integrals and \(W_m\) remain. The latter also becomes a bounded-interval moment: \[ W_m(2n)=\frac1{4\pi}\int_0^{w_0} s^{n-1}e^{\pi m}s^{m/2}\,ds, \qquad w_0=e^{-2\pi}. \] The elementary polynomial differences are \[ \begin{array}{c|c|c|c} \text{parity of }m&p(t)&\delta_m p& U_m[p]+\dfrac{\delta_m p}{2\sigma_m}V_m^{(d)} \\ \hline \text{even}&1&0&U_{m,0}\\ \text{even}&t&0&U_{m,1}\\ \text{even}&t^2&2&U_{m,2}+V_m^{(d)}\\ \text{odd}&1&4&U_{m,0}-2V_m^{(d)} \end{array} \] These are precisely the four coefficient families used in the paper. Among polynomial weights, the requirement that \(\delta_m p\) be constant permits degree at most two for even \(m\), and degree zero for odd \(m\). For even \(m\), the difference kills constants and linear polynomials, and sends degree \(k\geq2\) to degree \(k-2\); for odd \(m\), it preserves the leading degree. Higher-degree weights could be considered, but their real-path terms would require additional reciprocal families for this cancellation. \subsection{What the calculation explains} The construction now has a sequence of reasons: the lattice nodes suggest \(P\); inversion of Gaussians pairs the two integration ranges; exponential modes organize the unknowns into series; and the polynomial difference calculation leaves three even series and one odd series. The resulting Fourier values and derivatives become two moment families on fixed supports. Their two Cauchy transforms, together with the four generating series, account for the six functions in the boundary and bundle problems. These observations motivate a tractable coefficient space. They neither characterize every family with the prescribed zeros nor prove that the chosen system has a nonzero solution. Existence and uniqueness require the continuation, index, and vanishing arguments in the body of the paper. The later comparison with the known magic functions confirms which function this construction produces; it is not used to justify the choices in this appendix. \section{A compact regularizing operator}\label{app:K} For completeness we specify the operator used in Section~\ref{sec:operator}. The construction turns the local continuation proof into a bounded linear operation on arbitrary coefficient vectors, including vectors that do not solve the equations. For arbitrary \(\mathbf c\in\ell^2(\mathcal I_{24})\), use \eqref{eq:measures} and \eqref{eq:Cauchy} to define \(\mathbf h\) and \(\mathbf h_{\mathrm{par}}\) on the same interior domains. No vanishing of the exterior Cauchy function is needed for these definitions. For a center \(\zeta_0\in\mathbb C\), a radius \(r>0\), and an area-integrable function \(h\) on the disk \(D(\zeta_0,r)\), define its holomorphic average by \begin{equation} (\mathsf B_{\zeta_0,r}h)(z)=\frac1{\pi r^2} \int_{D(\zeta_0,r)} \frac{h(\zeta)} {(1-(z-\zeta_0)\overline{(\zeta-\zeta_0)}/r^2)^2}\,dA(\zeta). \label{eq:Bergman} \end{equation} For \(0<\sigma<1\), \[ \sup_{|z-\zeta_0|\leq\sigma r}|\mathsf B_{\zeta_0,r}h(z)| \leq\frac{\|h\|_{L^1(D(\zeta_0,r))}}{\pi r^2(1-\sigma)^2}. \] Expanding the kernel and integrating angularly proves that \(\mathsf B_{\zeta_0,r}\) reproduces every holomorphic area-integrable function on the disk. The continuation formulas will first assign functions separately on open pieces. For arbitrary coefficient vectors those assignments need not agree across the separating curves. We denote them by the subscript \(\mathrm{raw}\), and use a superscript \(\sharp\) for the holomorphic functions obtained by applying \(\mathsf B\). Values on the separating curves do not affect the area integrals. \begin{enumerate} \item On \(\{|z-1|<1/4,\ |z|>1\}\), assign functions \(b_{\mathrm{end},\mathrm{raw}},b_{-,\mathrm{raw}}\) from \eqref{eq:localHX} where \(\Re z>1\), from the first identity of \eqref{eq:local-lenses} in the lower left lens, and from the second in the upper left lens. Inside \(|z|<1,\ |z-1|<1/8\), assign \[ b_{\mathrm{end},\mathrm{raw}}(z)=z^{10}b_{\mathrm{end},\mathrm{raw}}(1/z),\qquad b_{-,\mathrm{raw}}(z)=b_{\mathrm{end},\mathrm{raw}}(z)-z^{10}b_{-,\mathrm{raw}}(1/z). \] Apply \(\mathsf B_{1,1/8}\) to get \(b_{\mathrm{end}}^\sharp,b_-^\sharp\). \item For \(z\in D(1,1/8)\) with \(\Re z>1\), set \(b_{+,\mathrm{raw}}(z)=\Aplus(Q(z))\). For \(\Re z<1\), use the expression in \eqref{eq:localXplus}. Apply \(\mathsf B_{1,1/8}\) to obtain \(b_+^\sharp\), and define \[ a_{2,\mathrm{par}}^\sharp(z)=(b_+^\sharp(z)+b_-^\sharp(z))/2,\qquad a_{3,\mathrm{par}}^\sharp(z)=(b_+^\sharp(z)-b_-^\sharp(z))/4. \] These averaged functions have argument \(z\), whereas the original \(A_j\) have argument \(q\). For an exact coefficient solution their relation is \(a_{j,\mathrm{par}}^\sharp(z)=A_j(Q(z))\). \item For \(z\in D(1,1/32)\) with \(\Re z>1\), set \(a_{1,\mathrm{par},\mathrm{raw}}(z)=A_1(Q(z))\). On the two left half-disks use \eqref{eq:localA1}, with the sharp functions in place of \(b_{\mathrm{end}},A_2,A_3\). Apply \(\mathsf B_{1,1/32}\) to get \(a_{1,\mathrm{par}}^\sharp\), and use \eqref{eq:localA0} to define \(a_{0,\mathrm{par}}^\sharp\). Write \(\mathbf a_{\mathrm{par}}^\sharp=(a_{0,\mathrm{par}}^\sharp,a_{1,\mathrm{par}}^\sharp,a_{2,\mathrm{par}}^\sharp,a_{3,\mathrm{par}}^\sharp)^T\). \end{enumerate} \paragraph{Bounds for arbitrary coefficients.} These estimates use no matching identity. In the first two stages, Lemma~\ref{lem:local-area} bounds the Cauchy pieces, the original series pieces, and their pullbacks by inversion. In particular \[ \|b_{\mathrm{end},\mathrm{raw}}\|_{L^1(D(1,1/8))} +\|b_{-,\mathrm{raw}}\|_{L^1(D(1,1/8))} +\|b_{+,\mathrm{raw}}\|_{L^1(D(1,1/8))} \leq C\|\mathbf c\|_2. \] The averaging estimate bounds the three sharp functions, and hence \(a_{2,\mathrm{par}}^\sharp,a_{3,\mathrm{par}}^\sharp\), on \(D(1,1/16)\) by \(C\|\mathbf c\|_2\). In the third stage these functions are consequently bounded on all of \(D(1,1/32)\). The remaining terms in \eqref{eq:localA1} are Cauchy pieces on the left and the original series on the right. Lemma~\ref{lem:local-area} therefore gives \[ \|a_{1,\mathrm{par},\mathrm{raw}}\|_{L^1(D(1,1/32))} \leq C\|\mathbf c\|_2. \] A second application of the averaging estimate, followed by \eqref{eq:localA0}, yields \[ \sup_{|z-1|\leq1/64}\|\mathbf a_{\mathrm{par}}^\sharp(z)\|_1 \leq C_0\|\mathbf c\|_2. \] These are bounds for the piecewise raw assignments of an arbitrary vector, not conclusions about its analytic continuation. \paragraph{Reproduction for exact solutions.} If \(\mathbf c\in\ker\Mom\), the overlap checks and removals in Proposition~\ref{prop:regularity} show that each raw assignment is the restriction of the actual holomorphic continuation. Disk averaging reproduces it. The first two stages therefore recover \(b_{\mathrm{end}},b_\pm\) and \(A_2(Q(z)),A_3(Q(z))\); the third recovers \(A_1(Q(z))\) and then \(A_0(Q(z))\). Thus \(\mathbf a_{\mathrm{par}}^\sharp(z)= \mathbf a_{\mathrm{ser}}(Q(z))\) for an exact solution. This reproduction statement is separate from the arbitrary-input bounds above. \paragraph{Coefficient extraction.} Put \(R=e^{\pi2^{-19}}\), \(\sigma_0=1-2^{-19}\), \(\delta_{\mathrm{end}}=2^{-7}\), and \(\mathsf S_{\mathrm{par}}=\operatorname{diag}(1,1,1,-1)\). Here \(\mathsf S_{\mathrm{pair}}\) is the paired-trace matrix of \eqref{eq:paired-transfer}, and \(\mathsf S_{\mathrm{par}}\) records the parity of the four series. Define paths \(z_R(t)=\sigma_0+it\) and \(\gamma_R(t)=Re^{-\pi it}\), \(0\leq t\leq1\). Then \(Q(z_R(t))=\gamma_R(t)\), and \(\gamma_R\) parametrizes the lower semicircle in the \(q\)-plane from \(R\) to \(-R\). Define a vector-valued function on this semicircle by \[ \widetilde{\mathbf a}_{\mathrm{ser},\mathbf c}(\gamma_R(t))= \begin{cases} \mathbf a_{\mathrm{par}}^\sharp(z_R(t)),&0\leq t<\delta_{\mathrm{end}},\\ \mathsf S_{\mathrm{pair}}(z_R(t))^{-1} \begin{pmatrix}\mathbf h_{\mathrm{par}}(z_R(t))\\\mathbf h_{\mathrm{par}}(z_R(t)-i)\end{pmatrix}, &\delta_{\mathrm{end}}\leq t\leq1-\delta_{\mathrm{end}},\\ \mathsf S_{\mathrm{par}}\mathbf a_{\mathrm{par}}^\sharp(z_R(t)-i),&1-\delta_{\mathrm{end}}