\section{Weighted removal and spectral bounds}\label{sec:03-removal} This section collects the tools shared by the later sections. We first record two standard spectral results. We then state a lower bound for the Coulomb form on regions where the electrons are separated radially (Lemma~\ref{lem:regional-bound}). Finally we prove the criterion for nonbinding that Sections~\ref{sec:04-helium-dianion} and~\ref{sec:07-lithium-dianion} apply to the two dianions (Proposition~\ref{prop:quadratic-removal}). The first spectral result is the HVZ theorem. In the present normalization, its fermionic form is stated in \cite{nam2012}. \begin{theorem}[HVZ]\label{thm:hvz} For the operators in Set-up~\ref{setup:atoms}, every integer $N\geq2$ and every $Z>0$ satisfy \[ \sigma_{\mathrm{ess}}(\AtomH{N}{Z})=[\AtomE{N-1}{Z},\infty). \] \end{theorem} The second spectral result is the spectrum of the hydrogenic operator. The formula below uses the Hartree kinetic coefficient $1/2$. \begin{theorem}[Hydrogenic spectrum]\label{thm:hydrogen} For $Q>0$, let $h_Q=-\Delta/2-Q/|x|$ be the scalar Coulomb operator on $L^2(\mathbb R^3)$. Its negative eigenvalues are $-Q^2/(2n^2)$, $n\in\mathbb N$, with spatial multiplicity $n^2$, and its remaining spectrum is $[0,\infty)$. If $P_m$ projects onto the shells $1\leq n\leq m$, where $m\geq1$ is an integer, then \[ h_Q\big|_{(1-P_m)L^2}\geq-\frac{Q^2}{2(m+1)^2}. \] \end{theorem} This is \cite[Theorem~10.9]{teschl2009}, with its operator $-\Delta-\gamma/|x|$ taken at $\gamma=2Q$ and divided by two. After including spin, the first $m$ hydrogenic shells have dimension $2\sum_{n=1}^m n^2$. Both dianion proofs need lower bounds for the Coulomb form on regions where some electrons are confined to a ball and the others are kept outside a larger ball. We call the confined electrons core electrons and the others outer electrons. The following lemma collects these bounds. It uses no symmetry of the test function. \begin{lemma}[Regional lower bound]\label{lem:regional-bound} Let $2\le N\le9$, $Z>0$, and let $\mathfrak h$ denote the Coulomb integral of Set-up~\ref{setup:atoms} with $N$ electrons and charge $Z$ on the full space $H^1((\mathbb R^3)^N;(\mathbb C^2)^{\otimes N})$, without symmetry restriction. For $-1\le z<1$ put $c(z)=\min\{1,[2(1-z)]^{-1/2}\}$ and $c(1)=1$, and let $D_0,\ldots,D_N$ be rational numbers with $D_0=D_1=0$ and \[ D_h\le\binom h2\sqrt{\frac{h-1}{2h}}\qquad(2\le h\le N); \] the values used in this paper are \[ (D_0,D_1,D_2,D_3,D_4,D_5) =\left(0,0,\frac12,\frac{433}{250},\frac{1837}{500},\frac{1581}{250}\right), \] whose squares for $h=3,4,5$ are below the exact values $3,27/2,40$. Fix $R,b,\lambda>0$, $\sigma\ge1$, an integer $0\le j\le N-1$, and set \[ \kappa=\lambda\sigma^2,\qquad C=\frac{\lambda^2}{2}+\frac{\lambda(\sigma-1)^2}{R},\qquad A_j=Z-\kappa-\frac{jR}{R+b}, \] \[ M_j(R,b,\lambda,\sigma) =\frac{jZ^2}{2}+(N-j)C+\frac1R\max_{0\le h\le N-j}\bigl(A_jh-D_h\bigr). \] If a spinor $v\in H^1$ is supported where $j$ specified electrons have radii below $b$ and the other $N-j$ have radii above $R$, then \[ \mathfrak h[v]\ge-M_j(R,b,\lambda,\sigma)\,\|v\|^2 . \] For $j=0$ the parameter $b$ is immaterial. \end{lemma} \emph{Idea of the proof.} The repulsion among the outer electrons is bounded below in terms of their directions. Each outer electron then satisfies a one-dimensional radial inequality, and each core electron is bounded by its hydrogenic ground energy. The full proof is in Appendix~\ref{sec:13-deferred-proofs-regional}. The increments $D_{h+1}-D_h$ of the listed values are $0,\frac12,\frac{308}{250},\frac{971}{500},\frac{53}{20}$. Hence the maximum defining $M_j$ is attained at $h=2$ whenever $\frac12\le A_j\le\frac{308}{250}$, which is the case for every parameter choice below. We now state the criterion for nonbinding. Its proof follows Lieb's argument for the bound $N<2Z+1$~\cite{lieb1984}. Lieb tests the eigenvalue equation against the eigenfunction multiplied by the radius of one electron, and bounds the energy of the other $N-1$ electrons from below by the threshold. We use the quadratic weight $r_i^2+\beta$ in place of the linear one. We also add correction terms $B_j$. They use the hypothesis that every state with at most $j-1$ electrons within the radius $b_j$ has energy at least $d_j$ above $U$. We call $d_j$ an exterior gap. \begin{proposition}\label{prop:quadratic-removal} Let $N\geq2$, $Z>0$, $\beta>0$, $U\geq\AtomE{N-1}{Z}$, and let $J\subset\{1,\ldots,N\}$ be finite. For $j\in J$ let $b_j,d_j>0$ and $\lambda_j\geq0$. Assume \[ \mathfrak q_{N,Z}[v]-U\|v\|^2\geq d_j\|v\|^2 \] in the quadratic-form sense for every fermionic form-domain vector $v$ vanishing almost everywhere on $\{q_j\leq b_j\}$. For $s\geq0$ define \[ B_j(s)=(s-b_j)_+^2-\frac{\min\{s/b_j,1\}}{2d_j}. \] For compactly supported fermionic $u\in H^1$ define \begin{align*} M_{\beta,U}[u]={}&\frac12\sum_i\int(r_i^2+\beta)|\nabla_i u|^2\\ &+\int\left[\sum_{i0$ satisfies \[ M_{\beta,U}[u]+\sum_{j\in J}\lambda_j\int B_j(q_j)|u|^2 \geq\varepsilon\|u\|^2 \] for every such $u$, then $\AtomE{N}{Z}=\AtomE{N-1}{Z}$ and $\AtomH{N}{Z}$ has no nonzero $L^2$ eigenfunction at any energy at or below $\AtomE{N-1}{Z}$. \end{proposition} \begin{proof} Put $T=\AtomE{N-1}{Z}$ and suppose that $\AtomH{N}{Z}\Psi=E\Psi$, with $E\leq T\leq U$ and $\|\Psi\|=1$. Write $X=(x_1,\ldots,x_N)$ and let $\nabla$ denote the full gradient in $X$. \emph{Ordered-radius moments.} Fix $j\in J$. Outside the null set of tied or zero radii, the function $q_j$ agrees locally with one of the $r_i$. Hence $q_j$ is symmetric and Lipschitz, with $|\nabla q_j|=1$ almost everywhere. For $L>0$ set $g_L=\min\{(q_j-b_j)_+,L\}$. Both $g_L\Psi$ and $g_L^2\Psi$ belong to the fermionic form domain. Testing the eigenvalue equation with $g_L^2\Psi$ and expanding the gradient gives \[ \mathfrak q_{N,Z}[g_L\Psi]-E\|g_L\Psi\|^2 =\frac12\int|\nabla g_L|^2|\Psi|^2. \] Since $g_L\Psi$ vanishes on $\{q_j\leq b_j\}$ and $E\leq U$, the assumption of the proposition bounds the left side below by $d_j\|g_L\Psi\|^2$. On the right side, $|\nabla g_L|^2=\mathbf1_{\{b_j0$, a contradiction. Hence no eigenvalue at or below $T$ exists. The HVZ theorem (Theorem~\ref{thm:hvz}) gives $\AtomE{N}{Z}\leq T$ and makes any spectral infimum below $T$ an eigenvalue. It follows that $\AtomE{N}{Z}=T$. \end{proof}