Plectis Atlas
Search

↑ and ↓ move, Enter opens, Esc closes.

Reading view

Generalized ionization energies for full Coulomb atoms

OpenAI, 24 September 2026

PDFTeX source

Part of family 263: The ionization and generalized ionization conjectures. Read it with its family

This page is converted from the paper’s TeX source. Atlas reconstructs statement numbers from the paper’s typesetting source (TeX). Use the original PDF if they differ. One figure is shown as a placeholder; see the PDF for it.

Abstract

We prove the energy part of the generalized ionization conjecture for full nonrelativistic Coulomb atoms with two electron spin states. The energy needed to remove m electrons is asymptotic to a_{\TF}m^{7/3} whenever m\to\infty and Z/m\to\infty, with the Thomas–Fermi constant in atomic units. We also obtain both conjectured iterated limits.

1 Introduction

The ionization energy of an atom measures the cost of removing electrons while leaving its nucleus fixed. The first few electrons removed belong to the outer part of the atom, whereas the leading total energy is largely determined by the much denser inner region. Thomas–Fermi theory, introduced by Thomas and Fermi [15, 3], describes the leading large-charge energy. Lieb and Simon established this connection to the many-body Schrödinger theory [6, 7]. Their energy theorem [7, Theorem III.1] concerns terms of order Z^{7/3}. Subtracting two such total-energy asymptotics does not control a much smaller ionization energy: the remainder may exceed the difference being sought.

The generalized ionization conjecture asserts that Thomas–Fermi theory nevertheless determines the leading cost of removing many outer electrons, provided their number remains small compared with the nuclear charge. Solovej formulated this statement through upper and lower large-Z limits, followed by a large removed-electron-number limit [14, Section 3, Equation (1)]. We prove its energy part for the full two-spin Coulomb Hamiltonian, in the stronger joint regime in which both the number removed and the ratio of nuclear charge to that number tend to infinity.

Earlier full-model estimates cover different ionization regimes. Seco, Sigal and Solovej bounded the first ionization energy of a neutral atom by CZ^{20/21}, using the improvement recorded in their note added in proof [11, Theorem 1 and p. 315]. Ivrii’s estimates imply agreement with the magnitude of the Thomas–Fermi chemical potential for successive one-electron ionization energies of positive atoms when Z^{5/7}=o(Z-N) and Z-N=o(Z), where N is the number of electrons [4, Theorem 6.2.1]. These results leave open the joint neutral-to-positive-ion energy asymptotic addressed here.

Uniform excess-charge bounds were proved in Thomas–Fermi–von Weizsäcker theory by Benguria and Lieb [1]; Solovej proved uniform ionization bounds in reduced Hartree–Fock theory [12] and then in unrestricted Hartree–Fock theory [13]. The Thomas–Fermi–von Weizsäcker and Hartree–Fock results concern different variational problems. The passage to arbitrary correlated fermionic states requires additional screening estimates, obtained here through conditional many-body states.

1.1 The theorem and its normalization

In atomic units, let Z be a positive integer and let

H_{Z,N} =\sum_{i=1}^N\left(-\frac12\Delta_i-\frac{Z}{|x_i|}\right) +\sum_{1\le i<l\le N}\frac1{|x_i-x_l|} \tag{1.1}

act on \bigwedge^N L^2(\R^3;\C^2). Write E_Z(N)=\inf\sigma(H_{Z,N}) and E_Z(0)=0. For integers Z>m\ge1, define

I_m(Z)=E_Z(Z-m)-E_Z(Z).

The kinetic coefficient of the corresponding Thomas–Fermi functional is T=\frac3{10}(3\pi^2)^{2/3}. More explicitly, put

\mathcal T_Z(\rho) =T\int_{\R^3}\rho^{5/3} -Z\int_{\R^3}\frac{\rho(x)}{|x|}\,dx +\frac12\iint_{\R^3\times\R^3} \frac{\rho(x)\rho(y)}{|x-y|}\,dx\,dy,

and let E_Z^{\TF}(N) be its infimum over nonnegative densities of mass N and finite displayed terms. Set I_m^{\TF}(Z)=E_Z^{\TF}(Z-m)-E_Z^{\TF}(Z). The constant in the conjecture is characterized by the classical Thomas–Fermi weak-ionization law [2, Section 6, Corollary 5]:

\lim_{Z\to\infty}I_m^{\TF}(Z)=a_{\TF}m^{7/3},\qquad m>0. \tag{1.2}

Our identification of the coefficient in Section 6 recovers this characterization in the present normalization.

Theorem 1.1 (Generalized ionization energy). For full nonrelativistic Coulomb atoms with two electron spin states,

\frac{I_m(Z)}{m^{7/3}}\longrightarrow a_{\TF}>0 \quad\text{whenever}\quad m\longrightarrow\infty, \qquad \frac Zm\longrightarrow\infty, \tag{1.3}

where Z>m\ge1 are integers. In particular,

\begin{align*} \lim_{m\to\infty} \frac{\limsup_{Z\to\infty} I_m(Z)}{m^{7/3}} &=a_{\TF},\tag{1.4}\\ \lim_{m\to\infty} \frac{\liminf_{Z\to\infty} I_m(Z)}{m^{7/3}} &=a_{\TF}. \tag{1.5}\end{align*}

The inner limits are taken over integer Z with m fixed. No convergence of I_m(Z) at a fixed m is asserted or assumed.

The limits in Equations (1.4) and (1.5) are precisely the energy part of the generalized ionization conjecture formulated by Solovej [14, Section 3, Equation (1)]. The joint assertion Equation (1.3) strengthens that order of limits. For historical comparison, Solovej established uniform first-ionization upper bounds and sharp generalized radius estimates in unrestricted Hartree–Fock theory [13, Theorems 3.8 and 1.5]; the generalized conjecture and its Hartree–Fock history are discussed in [14, Section 3]. Here the energy is the exact spectral infimum of Equation (1.1), with no restriction to Slater determinants.

For this same full two-spin Coulomb model, the companion [9, Corollary 1.3] also proves 0<c\le E_Z(Z-1)-E_Z(Z)\le C<\infty uniformly for every integer Z\ge1. This first-ionization bound does not assert convergence at fixed m and is distinct from the large-m limits above.

1.2 A price per electron

The proof first allows the particle number to vary. For fixed Z, abbreviate E_n=E_Z(n), and introduce the unconstrained energy and the priced minimum

E=\inf_{n\ge0}E_n,\qquad P(\lambda)=\min_{n\ge0}\bigl(E_n+\lambda n\bigr),\qquad\lambda>0.

The minimum exists, as verified in Section 2. Its advantage is local: replacing the exterior electrons by a trial state need not preserve their number. The price accounts for the change exactly. At the length scale s=\lambda^{-1/4}, the removed charge is of order s^{-3}. The main intermediate result identifies its coefficient for every minimizing sector, including at prices where several sectors minimize.

Theorem 1.2 (Deficit at a prescribed price). There is a universal number q>0 such that, for every sequence satisfying

\lambda=s^{-4},\qquad s\longrightarrow0, \qquad Zs^3\longrightarrow\infty,

and every choice of n minimizing E_n+\lambda n, one has

s^3(Z-n)\longrightarrow q.

The number q is the exterior Coulomb charge of the unique classical solution, tending uniformly to zero at infinity, of

\Delta F=4\pi k\bigl((F-1)_+\bigr)^{3/2} \quad\text{on }\R^3\setminus\{0\}, \qquad k=(5T/3)^{-3/2},

that is bounded above and below by positive multiples of |x|^{-4} near zero. The density k((F-1)_+)^{3/2} has bounded support, and F(x)=q/|x| outside that support. Moreover,

a_{\TF}=\frac37q^{-4/3}.

1.3 Analytic precedents and proof structure

The local kinetic comparison combines two classical constructions. Coherent wave packets provide the upper semiclassical energy [5, Section V.A.1]; see also [13, Lemma 8.2]. Neumann cube eigenvalues and their lattice count supply a lower comparison with the same leading coefficient [7, Theorems III.10–III.13]. Their remainders are controlled by local particle counts. This is different from the coarse Lieb–Thirring kinetic inequality [8], whose positive universal constant is sufficient for preliminary density bounds; the spectral splitting proof used in the companion follows Rumin [10, Theorem 1.4 and Section 3.1].

Screened exterior potentials and outward Thomas–Fermi comparisons are central to Solovej’s Hartree–Fock argument [13, Sections 6, 10, and 12]. Our use of conditional states requires a separate transfer from local quantum energies to conditional fields, while accounting for changes in particle number. The eventual singular profile belongs to the classical Sommerfeld comparison theory [7, Section IV], including the nonspherical comparisons and chemical-potential estimates of [13, Lemma 4.4, Remark 4.5, Theorem 4.6, and Corollary 4.7]. The issue here is to obtain that profile from the correlated quantum state and preserve its positive singularity through conditioning.

We use the localization, screening, and Thomas–Fermi estimates proved in the companion Uniform excess charge for Coulomb molecules and the outer radius of neutral atoms [9]. In particular, its uniform neutral-sector bound E_Z(Z)-E\le C fixes the zero-price integration constant, and its local-field estimates retain explicit control of an arbitrary energy offset [9, Proposition 12.3 and Proposition 4.5]. The required positive-price conditional comparisons and barrier propagation are proved in Sections 3 and 4. Their offset dependence is essential: a minimizing priced state has energy at most E+Cs^{-7}, so the allowed offset grows as s\to0. A fixed-offset conclusion from the neutral-atom theory cannot by itself yield Theorem 1.1.

Section 2 obtains the rough deficit bound and proves that the rescaled exterior electron mass vanishes beyond a fixed radius. In Section 3, noisy observations of the electrons permit local conditional comparisons while controlling the cost of conditioning. A Thomas–Fermi trial state in a small ball is compared with the priced many-body state. A fresh spatial cut records the local particles and leaves a core outside the patch, whose conditional screened potential is harmonic on the patch. Matching this core comparison to the noisy-observation law yields simultaneous upper and lower implications between local density and local potential. Two posterior laws occur in this argument; keeping them distinct is necessary for the Coulomb comparison.

The remaining difficulty is to retain the singular inner charge through successive averaging. Section 4 constructs a positive subsolution at the innermost scale and propagates it through the observation scales. The construction pays for exceptional conditional data with an error density of vanishing expected mass. The weak differential inequality is proved on open neighborhoods of the retained branches before taking their maximum, so no derivative is restricted to an activity interface. Section 5 then selects conditional data, rescales by s, and obtains a decaying solution of the unit-price Thomas–Fermi equation. The barrier prevents loss of the singularity. A maximum-principle argument identifies its Sommerfeld coefficient and proves uniqueness, which forces the same deficit for every minimizing sector.

Finally, Section 6 integrates the slopes of the priced minimum and brackets the desired particle number between two minimizing sectors. Only monotonicity of E_Z(N) is used in this step; convexity in N is not needed. The analogous Thomas–Fermi calculation identifies the coefficient with Equation (1.2). A sequential argument then gives the specified order of limits in Equations (1.4) and (1.5).

2 Priced sectors and an exterior cutoff

The price per electron permits insertion and deletion comparisons without a constraint on the exterior particle number. We first collect the screening estimates that remain applicable when the energy above the unpriced minimum grows. Throughout, write

K(x)=\frac1{|x|},\qquad V=ZK,\qquad \nu=Z\delta_0,\qquad D(f)=\frac12\iint_{\R^3\times\R^3} \frac{f(x)f(y)}{|x-y|}\,dx\,dy,

and use the constants

T=\frac3{10}(3\pi^2)^{2/3},\qquad k=\left(\frac{5T}{3}\right)^{-3/2}.

These are the Thomas–Fermi constants for two spin states and kinetic energy -\Delta/2. For a fixed integer Z, abbreviate E_n=E_Z(n), put E_0=0, and define

E=\inf_{n\ge0}E_n,\qquad P(\lambda)=\min_{n\ge0}(E_n+\lambda n)\quad(\lambda>0).

The existence of this minimum follows below. The asymptotic regime used until Section 6 is

\lambda=s^{-4},\qquad s\longrightarrow0, \qquad Zs^3\longrightarrow\infty. \tag{2.1}

Every assertion concerning a minimizing sector applies to every choice of minimizing index at every system in this regime.

If \psi is a normalized finite-sector form-domain vector, we call it an unshifted \delta-state when its form energy is at most E+\delta, where \delta\ge0. Its position law is |\psi|^2, with the spin variables summed unless they are recorded; its one-particle density is denoted by \rho_\psi. Expectations may also include the auxiliary random labels specified below. For a real number v, write v_+=\max(v,0) and v_-=\max(-v,0). Constants C,c>0 can change from line to line. Unless a dependence is displayed, they depend only on this fixed model and on the fixed cutoff and kernel conventions.

2.1 Imported estimates and their hypotheses

Lemma 2.1 (Sector and energy estimates). The sequence E_n is nonincreasing. If E_n<E_{n-1}, there is a normalized ground state in sector n, and n\le2Z+1\le3Z. There is a largest such index N_*, with Z\le N_*\le3Z, and

E=E_{N_*}=E_n\quad(n\ge N_*).

There are universal C,Z_0 such that

E_Z(Z)\le E+C\qquad(Z\ge Z_0). \tag{2.2}

If \Psi is a normalized sector ground state and F is a bounded real symmetric Lipschitz function of the spatial configuration, then

\langle F\Psi,H_{Z,n}F\Psi\rangle -E_n\|F\Psi\|_2^2 =\frac12\E_\Psi|\nabla F|^2, \tag{2.3}

where the left side is interpreted as a quadratic form and the gradient includes all spatial coordinates. Finally, every unshifted \delta-state in a sector n\le3Z satisfies

\int_{\R^3}\rho_\psi^{5/3}\le C(Z^{7/3}+\delta). \tag{2.4}

Proof. The sector assertions and the multiplier identity are [9, Lemmas 2.1 and 2.4–2.6]; the density estimate is [9, Lemma 3.3]. The stronger estimate E_Z(Z-1)\le E+C is [9, Proposition 12.3]. Monotonicity gives Equation (2.2). All these results use exactly the Hamiltonian and the two-spin convention fixed here.

A one-particle square cut consists of nonnegative bounded-gradient Lipschitz functions o,c with o^2+c^2=1. Conditional on the positions, assign the particles independently to the out and core groups with probabilities o^2 and c^2. The cut data record the out labels, positions, and spins. For a finite sequence of cuts, stage labels are recorded as well. Conditional core states are obtained by the corresponding products of cut factors, so antisymmetry is preserved within each group. This is the localization convention of [9, Lemma 3.4].

The local estimate needed for the later patch comparison has a quantitative condition on these cuts. Fix, once and for all,

L=10^5,\qquad A=40,\qquad a_y=|y|/L,\qquad B_y=B(y,a_y) \quad(y\ne0).

For an unshifted \delta-state put

\begin{gathered} m_y=\max(a_y^{-3},1)+\sqrt{\delta a_y},\qquad J_y=V(y)-\sum_{|x_i-y|\ge Aa_y}\frac1{|y-x_i|},\\ P_* =\max\left(1,\sup_{y\ne0} \frac{\E\bigl[\#\{i:x_i\in B_y\}^2\bigr]}{m_y^2}\right). \end{gathered}

The number P_* is finite for each finite system, since the count is at most the sector particle number and m_y\ge1.

Lemma 2.2 (Local fields for arbitrary offsets). For every normalized unshifted \delta-state of finite particle number, P_*\le C. Fix y\ne0 and C_0\ge1. The data X may be trivial. Otherwise, suppose that the initial cut, or finite sequence of cuts (o_h,c_h), has total out support covered by at most C_0 cells B_z with

C_0^{-1}\le a_z/a_y\le C_0, \qquad \sum_h\bigl(|\nabla o_h|^2+|\nabla c_h|^2\bigr) \le\sum_z D_z^2a_z^{-2}\ind_{B_z}, \qquad \frac{D_z^2}{a_zm_z}\le C_0\sqrt{P_*}.

Then, for the complete cut data,

\left\|(\E[J_y\mid X])_+\right\|_2 \le C(C_0)\frac{m_y}{a_y}. \tag{2.5}

The constants are independent of Z, the sector, the state, y, and \delta, apart from the displayed dependence through m_y.

Proof. This is [9, Proposition 4.5]. Its offset is measured from the minimum E over all sectors, just as here; it has no restriction that the offset stay bounded along a sequence. In all applications below we verify the stronger cut condition D_z^2/(a_zm_z)\le C_0.

Lemma 2.3 (Annular screening estimates). Let \psi be a normalized unshifted \delta-state of finite particle number. For fixed 0<\alpha<\beta<\infty and every u>0,

\left\|\#\{i:\alpha u\le|x_i|\le\beta u\}\right\|_2 \le C_{\alpha,\beta} \bigl(\max(u^{-3},1)+\sqrt{\delta u}\bigr). \tag{2.6}

Suppose in addition that n\le3Z, and set

B_{u/8}(x)=V(x)-\sum_{|x_i|<u/8}\frac1{|x-x_i|}.

Let Y be trivial or be the data of a square cut whose out support lies in \{u/4\le|x|\le8u\} and whose squared gradient sum is at most C/u^2. There are conditional versions harmonic on u/4<|x|<6u for which

\left\|\sup_{u/2\le|x|\le4u} \bigl(\E[B_{u/8}(x)\mid Y]\bigr)_+\right\|_2 \le C\left(\frac{\max(u^{-3},1)}u+\sqrt{\frac\delta u}\right). \tag{2.7}

The constant in the second estimate may depend on the fixed gradient bound. Both estimates allow every finite \delta.

Proof. The count estimate is [9, Corollary 4.9]. Boundary spheres have zero probability because the one-particle density is absolutely continuous, so open or closed annuli give the same estimate. For the field bound, use [9, Lemma 12.1] with inner cutoff h=u/8, broad annulus u/4<|x|<6u, and smaller annulus u/2\le|x|\le4u. The series in that lemma is

\frac{\max(u^{-3},1)+\sqrt{\delta u}}u +\sum_{j\ge0} \frac{\max((2^jh)^{-3},1)+\sqrt{\delta\,2^jh}} {\max(u,2^jh)}.

With h=u/8, geometric summation bounds it by the right side of Equation (2.7), also when u<1. The permitted cut support and gradient bound satisfy the fixed-annulus hypotheses of that lemma. The conditional harmonic versions follow by integration against the conditional law: for each fixed finite system the inner sources are uniformly separated from the annulus, so differentiation under the integral is valid. No minimizing property is required in either estimate.

2.2 The rough charge deficit

Lemma 2.4. The minimum P(\lambda) is attained. Along Equation (2.1), every minimizing index n is eventually nonzero and strictly bound. For a normalized ground state \Psi in that sector, put D_0=E_n-E. Uniformly over all these choices,

|Z-n|\le Cs^{-3},\qquad 0\le D_0\le Cs^{-7}. \tag{2.8}

Proof. By Lemma 2.1, E_n is constant for n\ge N_*. Since \lambda>0, the priced objective is strictly increasing thereafter, so its minimum is attained. If a minimizing index is positive, comparison with n-1 gives

E_{n-1}-E_n\ge\lambda>0.

It is therefore strictly bound, has a ground state, and satisfies n\le3Z. A normalized exponential one-electron trial of radius Z^{-1} has energy -Z^2/2. Moreover,

\frac\lambda{Z^2}=\frac{s^2}{(Zs^3)^2}\longrightarrow0.

Thus P(\lambda)<0 eventually, excluding the vacuum.

The neutral sector is an admissible competitor. By Equation (2.2),

0\le D_0\le C+s^{-4}(Z-n). \tag{2.9}

For a fixed inner configuration, the spherical average of B_{s/8} on |x|=s equals (Z-\#\{|x_i|<s/8\})/s. Its expectation is at least (Z-n)/s. Apply Equation (2.7) with trivial data and offset D_0 to obtain, for small s,

Z-n\le C\bigl(s^{-3}+\sqrt{D_0s}\bigr).

If d=Z-n\ge0 and z=s^3d, then Equation (2.9) gives D_0s^7\le Cs^7+z, whence

z\le C\bigl(1+\sqrt{z+Cs^7}\bigr).

This bounds z. If d<0, Equation (2.9) instead gives d\ge-Cs^4. These two cases prove the deficit estimate, and substitution in Equation (2.9) proves the bound for D_0.

2.3 A cutoff at one fixed exterior scale

Lemma 2.5. There is a sufficiently large fixed R_0 such that, for every sequence of minimizing sectors and corresponding ground states in Equation (2.1),

s^3\E_\Psi\#\{i:|x_i|>R_0s\}\longrightarrow0. \tag{2.10}

Proof. Choose a smooth 0\le\chi\le1 supported in [1/2,4] and equal to one on [1,2]. At shell scale u>0, write

w_i=\chi(|x_i|/u)^2,\quad S_u=\sum_iw_i,\quad m_u=\E S_u, \quad N_u=\E\#\{i:u/2\le|x_i|\le4u\}.

Test the weak eigen-equation with S_u\Psi. In its ith summand the other coordinates have energy at least E_{n-1}. Integration by parts gives for the selected-coordinate kinetic term

\frac12\operatorname{Re}\int\nabla_i\overline\Psi \cdot\nabla_i(w_i\Psi) =\frac12\int w_i|\nabla_i\Psi|^2 -\frac14\E\Delta_iw_i \ge-\frac14\E\Delta_iw_i.

Retain only the repulsions from particles in |x_l|<u/8; the selected particle lies outside that ball whenever w_i>0. Since E_{n-1}-E_n\ge s^{-4}, we obtain

s^{-4}m_u\le Cu^{-2}N_u +\E\sum_iw_iB_{u/8}(x_i). \tag{2.11}

All these tests are bounded symmetric form-domain multipliers for each fixed system.

Suppose m_u>0. Bias the position law by S_u/m_u, equivalently use the normalized state

\Psi_u=\sqrt{S_u/m_u}\,\Psi.

The function \sqrt{S_u} is the Euclidean norm of the vector of cutoffs. It is Lipschitz, including at its zeros, and

|\nabla\sqrt{S_u}|^2 \le Cu^{-2}\#\{i:u/2\le|x_i|\le4u\}.

The multiplier identity Equation (2.3) therefore makes \Psi_u an unshifted state of offset at most

\delta_u=D_0+Cu^{-2}N_u/m_u. \tag{2.12}

In both laws take the same auxiliary square cut, full out on u/2\le|x|\le4u, supported in u/4\le|x|\le8u, with gradient bounded by C/u. Its data Y determine S_u and every position with positive weight. Biasing by the Y-measurable variable S_u/m_u does not change the conditional raw law on S_u>0. Consequently the two conditional harmonic fields there are the same. Let

M(Y)=\sup_{u/2\le|x|\le4u} \bigl(\E[B_{u/8}(x)\mid Y]\bigr)_+

be this common conditional supremum. Conditioning first on Y gives

\E\sum_iw_iB_{u/8}(x_i) \le\E[S_uM(Y)] =m_u\E_{\Psi_u}M(Y).

The equality of conditional fields is used only on positive-bias data; zero-weight summands are omitted. Their harmonic continuity justifies evaluation at the recorded positions. Applying Equation (2.7) to \Psi_u, with Equation (2.12), now yields

\begin{align*} \E\sum_iw_iB_{u/8}(x_i) &\le Cm_u\left(\frac{\max(u^{-3},1)}u +\sqrt{D_0/u}\right) +Cu^{-3/2}\sqrt{m_uN_u}. \tag{2.13}\end{align*}

If m_u=0, the resulting shell estimate is immediate as well.

By Equation (2.8), for u\ge R_0s,

s^4\frac{\max(u^{-3},1)}u\le R_0^{-4}+s^4, \qquad s^4\sqrt{D_0/u}\le C\sqrt{s/u}\le CR_0^{-1/2}.

Choose R_0 large and then s small. The terms multiplying m_u in Equation (2.13) can be absorbed in Equation (2.11). As m_u\le N_u, the mixed term is at most Cu^{-3/2}N_u, and hence

m_u\le Cs^4(u^{-2}+u^{-3/2})N_u.

The annular count bound and Equation (2.8) also give

N_u\le C\bigl(u^{-3}+1+s^{-7/2}\sqrt u\bigr).

The shells on which the weights equal one, with u=2^jR_0s, j\ge0, cover the required exterior. Tonelli’s theorem and the two preceding inequalities give

\begin{align*} s^3\E\#\{|x_i|>R_0s\} &\le C s^7\sum_{j\ge0} (u^{-2}+u^{-3/2})(u^{-3}+1+s^{-7/2}u^{1/2}) \bigg|_{u=2^jR_0s}\\ &\le C_{R_0} \bigl(s^2+s^{5/2}+s^5+s^{11/2}\bigr) \longrightarrow0.\end{align*}

Every power of u in this sum is negative. Thus the estimate includes arbitrarily distant shells, with the same fixed R_0.

3 Conditional density and field comparison at positive price

We now obtain a local Thomas–Fermi relation for a conditional density. The conditioning retains information about the electron configuration while permitting a controlled change of state on any event of appreciable probability. Two different conditional laws enter the argument: observations define the density to be estimated, whereas a fresh spatial cut defines the core used in the energy comparison. We keep these laws separate and match their potentials only after taking expectation.

Throughout this section, \Psi is a normalized ground state in any sector n minimizing P(\lambda), with \lambda=s^{-4} and Equation (2.1) in force. In particular, n\leq 3Z and D_0=E_n-E\leq Cs^{-7} by Lemma 2.4. All statements about sufficiently small scales are uniform in the choice of this minimizing sector.

3.1 Nested observations and their energy cost

Fix 0<\eps<1, to be chosen in Section 4, and define

r_0=\eps Z^{-1/3},\qquad r_j=2^j r_0,\qquad J_* =\max\{j\geq0:r_j\leq s\},\qquad \ell_j=r_j^{1.01}\quad(0\leq j<J_*). \tag{3.1}

Eventually 2r_0\leq s. At each scale j<J_*, observe the unordered array of points x_i+\ell_jU_{ji}. All coordinates of all U_{ji} are independent, also independently of the raw configuration, with density

\zeta(u)=c_\zeta\exp\!\left(-\frac1{1-u^2}\right) \ind_{\{|u|<1\}}.

Labels are forgotten separately in each array. Let \mathcal F_j be the information in arrays j,\ldots,J_*-1, and let \mathcal F_{J_*} be trivial. These sigma-fields decrease with j.

Use the constants L=10^5, A=40 and a_y=|y|/L from Lemma 2.2. Fix a real radial function g\in C_c^\infty(B(0,1)) with \int g^2=1, set g_b(x)=b^{-3/2}g(x/b), and choose

w=10^{-5},\qquad 0<c_1<(10L)^{-1}.

Writing d_x=|x|, define the master packets and conditional fields by

\begin{aligned} D_x^{\mathrm b}&=\max(d_x,r_0),& t_x&=c_1D_x^{\mathrm b}\min(D_x^{\mathrm b},s)^w,\\ \mathcal K_x(y)&=g_{t_x}(y-x)^2,& \mu_j(y)&=\E\!\left[\sum_i\mathcal K_{x_i}(y) \,\middle|\,\mathcal F_j\right],\\ H'_j(y)&=V(y)-\lambda-(K*\mu_j)(y). \end{aligned} \tag{3.2}

The superscript \mathrm b indicates the lower clamp, not a power. The width function is globally Lipschitz, with \operatorname{Lip}(t)\leq c_1(1+w)s^w, and t_x\geq c_1r_0^{1+w}. Thus, for each fixed system, \mu_j is smooth in its evaluation variable, has mass n, and has deterministic bounds on all spatial derivatives. Its Coulomb potential and first derivatives are also continuous and deterministically bounded. These bounds at a fixed system will justify conditional integration; they are not claimed to be uniform in Z.

We use versions obtained by integrating against the conditional law of the raw configuration. Such versions can, for example, be specified by the finite-array likelihoods in [9, Lemma 5.1]. They give, simultaneously in space,

\E[\mu_j\mid\mathcal F_{j+1}]=\mu_{j+1},\qquad \E[H'_j\mid\mathcal F_{j+1}]=H'_{j+1},\qquad \Delta H'_j=-4\pi\nu+4\pi\mu_j. \tag{3.3}

Continuity extends identities first obtained on a countable dense set. In particular, H'_j is subharmonic off the nucleus.

Lemma 3.1 (Cost of an observation event). Let j<J_* and let A'\in\mathcal F_j have probability p>0. There is a normalized antisymmetric state \Psi_{A'} in the same sector whose raw law is the raw marginal conditioned on A' and whose form energy satisfies

\langle\Psi_{A'},H_{Z,n}\Psi_{A'}\rangle \leq E_n+C r_j^{-2.02}\log^5(e/p). \tag{3.4}

The constant is independent of the particle number, the number of observed arrays, and D_0.

Proof. If p_{A'}(x) is the probability of the observed event conditional on the raw positions, take \Psi_{A'}=\sqrt{p_{A'}(x)/p}\,\Psi. The multiplier is symmetric and preserves the form domain. The first inequality of [9, Lemma 5.2], with \ell_j=r_j^{1.01}, is exactly Equation (3.4). Its proof uses the ground-state multiplier identity in the sector n; it measures the cost above E_n, independently of the offset of E_n from E.

Accordingly, the unshifted offset of the tilted state is at most D_0+C r_j^{-2.02}\log^5(e/p), while its shifted energy is at most

P(\lambda)+C r_j^{-2.02}\log^5(e/p). \tag{3.5}

This distinction is what permits the local comparison below for D_0 up to order s^{-7}.

3.2 Statement and preliminary bounds

Proposition 3.2 (Simultaneous inverse comparison). There is a universal constant C_{\mathrm{cap}} with the following property. Fix

M\geq2,\qquad 0<h_l<h_h<\infty,\qquad 0<\xi<h_l/16.

For all sufficiently far systems along Equation (2.1), at every j<J_* there is an event \mathcal G_j\in\mathcal F_j such that, with r=r_j,

\Prob(\mathcal G_j^c)\leq Cr^{25}.

On \mathcal G_j, the following assertions hold simultaneously for r\leq d_y\leq4Mr and h_l\leq h\leq h_h:

\begin{split} d_y^4H'_j(y)&\leq C_{\mathrm{cap}},\\ d_y^6\mu_j(y)>kh^{3/2} &\quad\Longrightarrow\quad d_y^4H'_j(y)\geq h-\xi,\\ d_y^6\mu_j(y)<kh^{3/2} &\quad\Longrightarrow\quad d_y^4H'_j(y)\leq h+\xi. \end{split} \tag{3.6}

The probability constant and the threshold for sufficiently far systems may depend on the displayed fixed parameters and on the fixed packet conventions; C_{\mathrm{cap}} is independent of the band and accuracy parameters.

The two implications compare the field with each positive density height from opposite sides. They will yield an approximate Thomas–Fermi relation in Section 5, while permitting the field itself to be arbitrarily negative where the density is small.

We prove the proposition in the rest of this section. The proof uses the arbitrary-offset screening estimates from Section 2 and the energy cost in Lemma 3.1; it does not apply the fixed-offset inverse comparison of [9, Proposition 10.1] with a growing D_0.

Fix j<J_* and put r=r_j. On the enlarged band r/2\leq d_y\leq8Mr, write

a=a_y,\qquad t=t_y,\qquad \tau=t/a.

Uniformly there, for fixed M,

a\asymp_M r,\qquad c_Ma^w\leq\tau\leq Cs^w. \tag{3.7}

If \mathcal K_x(y)\ne0, the Lipschitz bound for the widths gives |x-y|\leq2t and t_x/t=1+O(s^w). Changing variables at scale t therefore gives

\int\mathcal K_z(y)\,dz=1+O(s^w). \tag{3.8}

On the local support, the kernel is bounded by Ct^{-3} and is Lipschitz, in either its center or its evaluation variable, with constant Ct^{-4}.

A count event. Except on an event of probability at most r^{40}, the jth observed array has at most C_Mr^{-3} entries in the radial band [r/4,12Mr]. To prove this, condition on the event that a sufficiently large such threshold is exceeded, if its probability is greater than r^{40}. Compact noise support forces every compatible raw configuration to have at least that many points in [r/8,13Mr]. By Lemma 3.1 and Equation (2.6), its conditional expected count is at most C_Mr^{-3}: indeed,

\sqrt{D_0r}\leq Cr^{-3}(r/s)^{7/2}\leq Cr^{-3},\qquad r^{-0.51}\log^{5/2}(e/r^{40})=o(r^{-3}).

This is a contradiction for a sufficiently large fixed threshold. Denote the retained event by \mathcal C_j. On it every compatible raw configuration has at most C_Mr^{-3} centers relevant to the enlarged band. Integration against the observation posterior consequently gives

0\leq\mu_j(y)\leq C_Mr^{-6-3w},\qquad |\nabla\mu_j(y)|\leq C_Mr^{-7-4w}. \tag{3.9}

A universal field cap. At a fixed point y of the enlarged band, condition on \{d_y^4H'_j(y)>b_0\} if it has probability p>0. Packets centered outside the exclusion ball in J_y do not contain y, by the width bound and the fixed choice of c_1. Their potentials at y equal the corresponding point potentials by radial averaging. Dropping the other nonnegative packet potentials and using the observation tower therefore bounds the event-mean of H'_j(y) above by the tilted mean of J_y-\lambda. The trivial-data case of Lemma 2.2 gives

b_0\leq C+C(d_y/s)^{7/2}-(d_y/s)^4 +C_Mr^{2.49}\log^{5/2}(e/p). \tag{3.10}

Here a<1 eventually. The polynomial-power difference on the right has a universal upper bound. Choose a universal C' exceeding the entire deterministic bound by one. Solving Equation (3.10) for p and integrating its stretched-exponential tail yields, for every fixed P>0,

\E\bigl(d_y^4H'_j(y)-C'\bigr)_+ \leq C_{P,M}r^P. \tag{3.11}

Subharmonicity turns this into a simultaneous bound. For 3r/4\leq d_y\leq6Mr, take a ball of radius d_y/10; it lies in the enlarged band. Its mean bounds H'_j(y) above. The contribution of C'd_z^{-4}, after multiplication by d_y^4, is bounded by a universal constant, and the remaining contribution is at most

Cr^{-3}\int_{\{r/2\leq d_z\leq8Mr\}} (d_z^4H'_j(z)-C')_+\,dz.

By Equation (3.11) and Markov’s inequality, the latter is at most one outside an event of probability C_Mr^{40}. We have proved the simultaneous cap

H'_j(y)\leq C_{\mathrm{cap}}d_y^{-4} \quad(3r/4\leq d_y\leq6Mr) \tag{3.12}

with a universal C_{\mathrm{cap}}.

3.3 A fine patch comparison with the price included

Fix a point y in the original band and a height h_l/2\leq h\leq2h_h. Suppose that one of the following events, intersected with \mathcal C_j, has probability p\geq r^{42}:

\begin{array}{ll} d_y^6\mu_j(y)>kh^{3/2},&d_y^4H'_j(y)<h-\xi/4,\\[2pt] d_y^6\mu_j(y)<kh^{3/2},&d_y^4H'_j(y)>h+\xi/4. \end{array} \tag{3.13}

Write Q for the original joint law conditioned on the event. When spatial cuts are introduced, enlarge this law by fresh labels with their ordinary conditional probabilities given the raw positions. Its raw marginal is the state from Lemma 3.1. Set

\delta'=Cr^{-2.02}\log^5(e/r^{42}),\qquad \delta=D_0+\delta'.

Then the raw state has unshifted offset at most \delta, shifted offset at most \delta', and

m_y\leq C_Ma^{-3},\qquad \delta'=o(a^{-6.98}). \tag{3.14}

The constants below may depend on the fixed band parameters.

Put \beta=a^{0.2} and b=\beta a, with s small enough that \beta<1/100. For each fixed band parameter M, the scales satisfy

b\ll\ell_j\ll t\ll a.

Here each ratio of consecutive scales tends to zero uniformly in j, also when r/s\to0, by Equation (3.7). The fine width b makes the semiclassical errors small; the broader master width t absorbs both this smearing and the observation displacement \ell_j, while t/a\to0 permits a local field comparison. The patch construction below has three outputs. Its energy comparison controls the Coulomb discrepancy and a negative-field penalty. The former, together with noisy-array matching, recovers the conditional density; the latter permits the high-density implication to pass to expectation. Finally, the two conditional-expectation identities recover the mean potential. We establish these transfers in that order.

Choose a square cut, using the sine and cosine of a smooth angle, that is full out on B(y,t_0), supported out in B(y,t_0+b), and has gradients bounded by C/b, where 5a\leq t_0\leq6a is selected below. Retain the out particles satisfying |x_i-y|<t_0-7b, and call the other out particles deleted. Let n_o denote the total number of out particles and n_{\mathrm{del}} the number of deleted particles; thus the retained count is n_o-n_{\mathrm{del}}. Then t_0 may be chosen so that

\E_Q n_o^2\leq C_Ma^{-6},\qquad \E_Q n_{\mathrm{del}}^2\leq C_M\beta a^{-6}. \tag{3.15}

For every candidate t_0, the total out count is bounded by the raw count in B(y,7a), which lies in a fixed annulus about the nucleus with radius comparable to a. The annular count estimate Equation (2.6), with Equation (3.14), bounds the expected square of this encompassing count by C_Ma^{-6}, uniformly in t_0. The deleted particles lie in the raw strip t_0-7b\leq|x_i-y|\leq t_0+b. Integrating its squared count over t_0\in[5a,6a], each ordered pair contributes for a set of lengths at most 8b. Averaging selects t_0 for the second bound in Equation (3.15), while preserving the first bound.

The fresh conditional core. In the cut marginal of the tilted state, let X record the out labels, positions, and spins. Slice only on these fresh cut data, not additionally on the noisy arrays. Denote the normalized core slice’s density by \rho_X^c and its energy, including the price per core electron, by e_X^\lambda. Then

e_X^\lambda\geq P(\lambda),\qquad \Phi=V-\lambda-K*\rho_X^c.

The localization products preserve antisymmetry within each group, and the normalized core slices are in their sector form domains for almost every datum [9, Lemma 3.4].

There is a nonnegative random variable F=F(X) such that

\Phi\leq F\text{ on }B(y,7a),\qquad \norm{F}_{L^2(Q)}\leq C_Ma^{-4}. \tag{3.16}

For this, condition the unshifted field obtained by subtracting only electrons outside B(y,20a); all those electrons belong to the core. This field is harmonic on B(y,10a) and bounds \Phi above there. At z\in B(y,10a), the inclusion B(y,20a)\subset B(z,Aa_z) bounds it above by \E_Q[J_z\mid X]. The cut satisfies Lemma 2.2 uniformly: a bounded number of comparable cells covers its out support, its gradient coefficients obey D_z^2\leq C\beta^{-2}, and a_zm_z\geq ca^{-2}, so that D_z^2/(a_zm_z)\leq Ca^{1.6}\leq C. That lemma bounds the positive part in L^2(Q) at each target z. Submeans on balls of radius a, followed by Minkowski’s integral inequality, give the positive supremum bound in Equation (3.16).

The patch minimizer. On \Omega=B(y,t_0-4b) minimize

\mathcal E_\Phi(f)=T\int f^{5/3}-\int\Phi f+D(f),\qquad f\geq0, \quad\supp f\subset\overline\Omega.

The field \Phi is bounded and harmonic on a neighborhood of \overline\Omega: the core is excluded from B(y,t_0), and the nucleus is far outside this patch. Coercivity in L^{5/3}(\Omega), weak lower semicontinuity, and strict convexity give a unique minimizer \rho=\rho_X. Its Euler equation is

W=\Phi-K*\rho,\qquad \rho=kW_+^{3/2}\text{ on }\Omega. \tag{3.17}

Nonnegative variations give the one-sided condition where \rho=0; variations of either sign on positive density give the equality. Comparison with zero and D(\rho)\geq(\int\rho)^2/(24a) show that

\int\rho\leq CaF. \tag{3.18}

These minimizers can be chosen measurably in X. One way to see this is to note their continuous dependence in L^{5/3} on a field in L^{5/2}(\Omega): coercivity bounds a converging sequence of minimizers; weak limits minimize the limiting functional by lower semicontinuity and comparison with its minimizer; uniqueness identifies the limit, and convergence of the minimum values forces convergence of the L^{5/3} norms. Uniform convexity gives strong convergence. The Coulomb form is a continuous positive quadratic form on L^{5/3}(\Omega), as used in this argument.

Let \vartheta_b be the radial probability kernel from [9, Lemma 3.6], obtained by averaging a cube kernel over translations and rotations. It is bounded by b^{-3} and supported in B(0,\sqrt3b). Define

\sigma=\sum_{i\ \mathrm{retained}}\vartheta_b(\,\cdot-x_i).

Every such smear lies in \Omega by the 7b retention margin. We claim

\E_Q\left[D(\sigma-\rho)+\int W_-\sigma\right] \leq C_Ma^{-7+.02},\qquad \int_{B(y,4a)}\rho_{\mathrm{tilt}}^{5/3}\leq C_Ma^{-7}, \tag{3.19}

where \rho_{\mathrm{tilt}} is the ordinary one-particle density of the tilted state. In particular, it is not the conditional patch density \rho.

Lower and upper energy comparisons. Write (o,c) for the fresh square cut and, for each out-label set I\subset\{1,\ldots,n\}, set

\Psi_I=\prod_{i\in I}o(x_i)\prod_{i\notin I}c(x_i)\Psi_{A'}, \qquad T_o=\frac12\sum_{I\subset\{1,\ldots,n\}}\sum_{i\in I} \norm{\nabla_i\Psi_I}_2^2.

Thus T_o is the total out kinetic energy in the localized state. Adding price to the exact localization identity of [9, Lemma 3.4] gives

\langle\Psi_{A'},H_{Z,n}\Psi_{A'}\rangle+\lambda n +\operatorname{err}_{\mathrm{loc}} =\E_Qe_X^\lambda+T_o -\E_Q\sum_{i\ \mathrm{out}}\Phi(x_i) +\E_Q\sum_{i<l\ \mathrm{out}}K(x_i-x_l), \tag{3.20}

with 0\leq\operatorname{err}_{\mathrm{loc}}\leq C_Mb^{-2}a^{-3}. The price has been included in the core energy and in \Phi; there is no localization error associated with it. [9, Lemma 3.6] allows any measurably selected retained subset and gives

\begin{split} T_o&\geq\E_Q\left[T\int\sigma^{5/3} -Cb^{-2}(n_o^{4/3}+n_o)\right],\\ \sum_{i<l\ \mathrm{out}}K(x_i-x_l)&\geq D(\sigma)-Cn_o/b. \end{split} \tag{3.21}

The leading kinetic coefficient here is exactly T, for two spin states and kinetic energy -\Delta/2.

For almost every fixed slice, the corresponding priced upper comparison is

P(\lambda)\leq e_X^\lambda+T\int\rho^{5/3} +Cb^{-2}\int\rho-\int\Phi\rho+D(\rho). \tag{3.22}

The coherent-packet construction is standard; see [13, Lemma 8.2]. We spell out why the insertion proof of [9, Lemma 3.5] also proves this priced version. Integrate the rank-one matrices of the orbitals g_b(x-z)e^{ip\cdot x}, for both spins, over |p|\leq(3\pi^2\rho(z))^{1/3} with measure dz\,dp/(2\pi)^3. The resulting one-body matrix \gamma satisfies

0\leq\gamma\leq1,\qquad \Tr\gamma=\int\rho,\qquad \rho_\gamma=g_b^2*\rho,

by Plancherel and momentum-ball integration. Its kinetic trace is

\Tr(-\Delta/2)\gamma=T\int\rho^{5/3}+Cb^{-2}\int\rho.

First truncate its spectral decomposition to finitely many eigenvectors. Occupy these independently with probabilities given by the eigenvalues. Every realization is a finite Slater determinant, with an integer number of electrons, and its mean repulsion is at most the direct energy of the truncated density by the direct-minus-exchange identity. Its support is in the packet region, which lies strictly inside B(y,t_0) and is separated from the core and nucleus. It may therefore be wedged with the core. Every resulting state has shifted energy at least P(\lambda), and the mean price paid by the inserted electrons is \lambda\Tr\gamma.

Positive spectral truncations have increasing densities and convergent traces. The potentials are bounded on the packet region for each fixed slice, so all one-body terms converge; direct energies converge by monotone convergence. Radial smearing does not increase D, and harmonic means replace \int\Phi(g_b^2*\rho) by \int\Phi\rho, including the constant price term. Averaging the integer-sector trials and passing to the limit proves Equation (3.22). This reasoning requires neither an integer value of \int\rho nor a measurable choice of a trial determinant as the slice varies.

For retained particles, harmonic means likewise give \sum_{i\ \mathrm{retained}}\Phi(x_i)=\int\Phi\sigma. The deleted attractions cost at most Fn_{\mathrm{del}}. Subtract Equation (3.22) in Equation (3.20), use Equations (3.5) and (3.21), and expand the functional about its minimizer. Convexity of the kinetic term leaves D(\sigma-\rho) and the linear term

\int\left(\frac{5T}{3}\rho^{2/3}-W\right)(\sigma-\rho) =\int W_-\sigma.

The equality uses Equation (3.17): where \rho>0 the coefficient vanishes, and where \rho=0 it equals W_-. By Equations (3.15), (3.16) and (3.18), the resulting bound is

\E_Q\left[D(\sigma-\rho)+\int W_-\sigma\right] \leq\delta'+C_M\left( \sqrt\beta\,a^{-7}+b^{-1}a^{-3} +b^{-2}(a^{-4}+a^{-3})\right). \tag{3.23}

All terms are integrable: for example, \int\rho\leq CaF and \mathcal E_\Phi(\rho)\leq0 bound both its kinetic and direct terms by CaF^2 in expectation. The exact cut identity also has integrable absolute Coulomb terms by form-domain admissibility.

Since b=a^{1.2}, the errors in Equation (3.23), divided by a^{-7}, are bounded by

C_M\left(a^{4.98}\log^5(e/a)+a^{.1} +a^{2.8}+a^{.6}+a^{1.6}\right).

This proves the first part of Equation (3.19). For the second, use e_X^\lambda\geq P(\lambda) directly in Equation (3.20). Dropping the nonnegative out repulsion and using \E_QFn_o\leq C_Ma^{-7} gives T_o\leq C_Ma^{-7}. The coarse kinetic-density inequality of [9, Lemma 3.4], on the full-out ball containing B(y,4a), proves the remaining assertion.

3.4 Recovering the conditional density from the patch

By Equation (3.17), the patch field satisfies \Delta W=4\pi kW_+^{3/2} on B(y,4a). We will use the bounds

W\leq Ca^{-4}\text{ on }B(y,3a),\qquad \sup_{B(y,2t)}|W-W(y)| \leq C\tau\bigl(a^{-4}+W(y)_-\bigr). \tag{3.24}

For the first, compare on the ball of radius R=4a with

U(x)=\frac{CR^4}{(R^2-|x-y|^2)^4}.

For large universal C, \Delta U\leq4\pi kU^{3/2}; it diverges at the boundary. Testing with the positive part of W-U proves the bound. For the second, the Coulomb potential of \rho\ind_{B(y,2a)} is O(a^{-4}) with gradient O(a^{-5}) on that ball, by the first bound and direct integration of the Coulomb kernel. Adding this potential to W leaves a harmonic function bounded above by Ca^{-4}. Apply the interior gradient estimate to its nonnegative harmonic distance from this upper bound. Its center value is at most Ca^{-4}+W(y)_-, which proves the oscillation estimate. These comparisons are classical or weak positive-part tests: compact L^{5/3} densities have continuous potentials, so W is continuous.

Define the local averaging operator

\mathcal R f(y)=\int\mathcal K_z(y)f(z)\,dz.

On every compatible path under Q, including its fresh cut labels,

|\mathcal R\sigma(y)-\mu_j(y)| \leq C_Mr^{-3}(\ell_j+b)t^{-4}=o(a^{-6}). \tag{3.25}

Here is the reason this comparison uses the original observation posterior correctly. Match any compatible raw configuration to the jth observed multiset. Each matched displacement is at most \sqrt3\ell_j, so the raw kernel sum is within C_Mr^{-3}\ell_jt^{-4} of the sum evaluated at that multiset. The same is true of its posterior average \mu_j at these data. Only C_Mr^{-3} entries can contribute, by \mathcal C_j. All relevant raw centers lie in the fully retained region of the fresh cut, since t/a\to0, b/a\to0, and \ell_j/a\to0. Replacing each such center by its fine smear changes the sum by at most C_Mr^{-3}bt^{-4}. This proves Equation (3.25) without identifying the two posterior laws. The ratios of these errors to a^{-6} are bounded by

C_M\bigl(a^{.01-4w}+a^{.2-4w}\bigr)=o(1).

Let

G=\{D(\sigma-\rho)\leq a^{-7+.01}\}.

By Equation (3.19), Q(G^c)\leq C_Ma^{.01}. The function z\mapsto\mathcal K_z(y) is a compactly supported Lipschitz test with gradient norm at most Ct^{-5/2}. Coulomb duality [9, Lemma 3.1] therefore gives, on G,

|\mathcal R\rho(y)-\mathcal R\sigma(y)| \leq Ca^{-7/2+.005}t^{-5/2}=o(a^{-6}). \tag{3.26}

Indeed the relative gain is at least a^{.005-(5/2)w}. All the small errors here are uniform for fixed parameters along Equation (2.1), including scales with arbitrarily small r/s.

On G, the high-density antecedent in Equation (3.13) forces

W(y)\geq(h-\xi/16)d_y^{-4}. \tag{3.27}

Otherwise Equation (3.24) would imply W(z)\leq(h-\xi/32)d_y^{-4} on the support of the averaging kernel. This remains true for arbitrarily negative W(y): its upper estimate contains the nonpositive term -(1-C\tau)W(y)_-. The Euler relation, Equation (3.8), and Equations (3.25) and (3.26) would then contradict the high-density antecedent. In the same way the low-density antecedent forces, on G,

W(y)\leq(h+\xi/16)d_y^{-4}. \tag{3.28}

The upper bound in Equation (3.24) lets Equation (3.28) pass to expectation with an o(a^{-4}) error.

The high case needs a bound on the negative field on G^c. The high antecedent and Equation (3.25) hold on all paths under Q, and give

\int_{B(y,2t)}\sigma\geq ca^{-6}t^3.

Using Equation (3.24) on this ball and absorbing C\tau W(y)_- yields

W(y)_-\leq C(a^{-6}t^3)^{-1}\int W_-\sigma+C\tau a^{-4}. \tag{3.29}

Consequently Equation (3.19) implies

\E_Q[\ind_{G^c}W(y)_-]=o(a^{-4}),

since the ratio of its bound to a^{-4} is at most C_Ma^{.02}\tau^{-3}+C\tau \leq C_Ma^{.02-3w}+Cs^w=o(1). Thus Equation (3.27) also passes to expectation with an o(a^{-4}) error. This step explicitly controls the negative part; no lower cap on the conditional field is assumed.

3.5 Matching the potentials of the two conditional laws

We adapt the averaged field transfer of [9, Lemma 5.3] to the present priced fields. The preceding patch estimates supply its required small errors; we give the two-law decomposition and estimates explicitly. We prove

\left|\E_Q\bigl(H'_j-W\bigr)(y)\right|=o(a^{-4}). \tag{3.30}

Write P^{\mathrm{raw}} and P^{\mathrm{ms}} for the raw and master-smeared electron potentials at y, and P^{\mathrm{ret}},P^{\mathrm{del}} for the raw potentials of retained and deleted out particles. Because the event defining Q is in \mathcal F_j, the original observation tower gives \E_Q(K*\mu_j)(y)=\E_QP^{\mathrm{ms}}. The core in W instead uses the fresh-cut tower in the tilted raw law. Combining these two identities, and cancelling both nucleus and price, expresses \E_Q(H'_j-W)(y) as the expectation of

(P^{\mathrm{raw}}-P^{\mathrm{ms}})-P^{\mathrm{del}} -(P^{\mathrm{ret}}-K*\sigma)(y)+K*(\rho-\sigma)(y). \tag{3.31}

By Hölder’s inequality and the ordinary density bound in Equation (3.19), for 0<u\leq4a the expected raw potential from B(y,u) is at most

\int_{B(y,u)}\frac{\rho_{\mathrm{tilt}}(z)}{|z-y|}\,dz \leq C_Ma^{-4}(u/a)^{1/5}. \tag{3.32}

Radial smearing never increases the potential of a point charge and leaves it unchanged outside the smear radius. The master-smearing difference in Equation (3.31) can therefore come only from centers within 2t of y; the fine-smearing difference can come only from centers within \sqrt3b. Equation (3.32) bounds both by o(a^{-4}). Deleted centers have distance comparable to a, so Equation (3.15) gives \E_QP^{\mathrm{del}}\leq C_Ma^{-4}\sqrt\beta.

For the remaining signed potential, truncate the kernel at height t^{-1}. The test z\mapsto\min(|z-y|^{-1},t^{-1}) has homogeneous Sobolev gradient norm O(t^{-1/2}). Coulomb duality, or its compactly supported approximation, and Equation (3.19) give expected absolute truncated error at most

C_Mt^{-1/2}a^{-7/2+.01}=o(a^{-4});

the relative gain is a^{.01}\tau^{-1/2}\leq C_Ma^{.01-w/2}. The truncation loss for \rho is at most Ca^{-6}t^2 by Equation (3.24). For \sigma, radial smearing and Equation (3.32) bound it by

C_Ma^{-4}\bigl((t+\sqrt3b)/a\bigr)^{1/5}.

These also vanish relative to a^{-4} by Equation (3.7). This proves Equation (3.30).

In the high case, Equations (3.27) and (3.29) give \E_QW(y)\geq(h-\xi/16)d_y^{-4}-o(a^{-4}), whereas the failed comparison in Equation (3.13) gives \E_QH'_j(y)\leq(h-\xi/4)d_y^{-4}. Equation (3.30) contradicts these inequalities eventually. The low case follows in the same way from Equation (3.28) and the upper bound on W. We conclude that each fixed-point failure in Equation (3.13), intersected with \mathcal C_j, has probability less than r^{42}.

3.6 Spatial and height nets

Take a spatial net of mesh at most r^2 in the original band, with O_M(r^{-3}) points, and a fixed finite height net in [h_l/2,2h_h] of mesh at most \xi/64. Exclude the fixed-point failures at all net pairs, the complement of \mathcal C_j, and the enlarged-cap failure. Their total probability is O_M(r^{39})+O_M(r^{40}), in particular at most Cr^{25}. All these events are \mathcal F_j-measurable.

The normalized density d_y^6\mu_j(y) changes by at most C_Mr^{1-4w}=o(1) between a point and its nearest net point, by Equation (3.9). For the field, work on balls of radius a small fixed multiple of r within the enlarged cap band. Adding the Coulomb potential of the local source \mu_j makes H'_j harmonic there and bounds that harmonic function above by C_Mr^{-4-3w}, using Equations (3.9) and (3.12). The positive-harmonic gradient argument used in Equation (3.24) shows that v(y)=d_y^4H'_j(y) varies over a displacement O(r^2) by at most

C_Mr^{1-3w}+C_Mr\,v(y)_-. \tag{3.33}

Suppose a high-density failure with tolerance \xi occurs at (y,h). If v(y)\geq0, Equation (3.33) puts the nearby net value below h-3\xi/4 for small s. If v(y)<0, the same upper estimate is bounded by (1-C_Mr)v(y)+C_Mr^{1-3w}, and gives the identical conclusion since h\geq h_l>16\xi. Choose a height-net value between h-\xi/4 and h-\xi/8. The small normalized-density variation preserves the strict high antecedent at this lower height, while the field value violates its comparison with tolerance \xi/4. This is an excluded net failure.

A low-density failure has v(y)>h+\xi>0. Its nearest net value is above h+3\xi/4 by Equation (3.33). A height-net value between h+\xi/8 and h+\xi/4 preserves the low antecedent and again yields an excluded failure with tolerance \xi/4. Thus both comparisons hold everywhere on the band for every h_l\leq h\leq h_h. Together with Equation (3.12), this proves Proposition 3.2.

4 Continuing a lower barrier

The local density–field comparison in Proposition 3.2 does not by itself exclude a limiting field which is too small near the nucleus. We now carry a positive barrier from the nuclear scale to an arbitrary intermediate scale. The construction keeps the actual conditional density inside the current radius and uses the Thomas–Fermi reaction outside it. Rare failures of the local comparison are retained as an explicit, small source error. This adapts the intermediate-subsolution construction of [9, Proposition 11.2], using the positive-price comparison proved here to allow the growing offset D_0=O(s^{-7}).

Write d=|y| and put

f(t)=4\pi k(t_+)^{3/2},\qquad b_r(y)=B d^{-4}\left(1-\frac r{8d}\right)\quad(d\ge r), \tag{4.1}

where B>0 will be fixed below. Direct differentiation gives

\Delta b_r=Bd^{-6}\left(12-\frac{20r}{8d}\right) \ge \frac{19}{2}Bd^{-6}.

Thus \Delta b_r\ge f(b_r) whenever 4\pi k\sqrt B\le19/2. If R=2r, then

b_r-b_R\ge\gamma R^{-4}\quad(R\le d\le1.1R), \qquad \gamma=\frac{B}{16(1.1)^5}>0. \tag{4.2}

Proposition 4.1 (Conditional barrier invariant). There are fixed positive constants \eps,B,C_{\mathrm{inv}} and M>2 with the following property. For every sufficiently far system in Equation (2.1), use the observations and kernels of Equations (3.1) and (3.2) with this \eps. For every 0\le j\le J_* there exist \mathcal F_j-measurable functions u_j,p_j such that, with r=r_j,

\begin{aligned} \Delta u_j&\ge-4\pi\nu +4\pi\ind_{\{d<r\}}\mu_j-4\pi p_j +\ind_{\{d\ge r\}}f(u_j),\\ b_r\le u_j&\le C_{\mathrm{inv}}d^{-4}\quad(d\ge r),\\ u_j&=b_r\quad(d>Mr). \end{aligned} \tag{4.3}

The first inequality holds in distributions on \R^3. For each fixed system, u_j-V is continuous and locally Lipschitz, with deterministic bounds on compact sets; p_j is a nonnegative bounded density supported in \{d\le r_j\}, also with a deterministic bound. Its expected total mass satisfies

\sup_{0\le j\le J_*}\E\int p_j \le C\bigl(r_0^{32}+s^{19/2-3w}\bigr)=o(1). \tag{4.4}

The deterministic fixed-system regularity bounds need not be uniform in Z; the constants in Equation (4.4) are uniform.

Proof. We use the weak maximum rule in [9, Lemma 5.4]. In its nonsingular form, if finitely many continuous locally H^1 functions satisfy

\Delta v_i\ge g(y)+F(y,v_i),

where g is locally bounded and F is measurable in y, continuous in its second variable, and locally bounded on bounded ranges, then their maximum satisfies the same inequality with its own value in the reaction. The lemma also allows a common singular term -4\pi\nu when all branches have continuous locally H^1 offsets from V and the reaction vanishes near the origin. These are the precise forms used below.

Initialization. For sufficiently small fixed \eps, the initial conditional density satisfies, outside an event of probability at most Cr_0^{35},

P_0(y):=K*(\ind_{\{d<r_0\}}\mu_0)(y) \le0.1\,Z/r_0 \quad(r_0\le |y|\le1.1r_0). \tag{4.5}

To prove this, fix y in the indicated annulus and consider the \mathcal F_0-event A_y=\{P_0(y)>0.05Z/r_0\}. If its probability is greater than r_0^{40}, Lemma 3.1 realizes its raw conditional marginal as a normalized state in sector n with unshifted offset at most

D_0+Cr_0^{-2.02}\log^5(e/r_0^{40}).

By Equation (2.8), D_0\le Cs^{-7}. Since r_0/s\to0, the displayed offset is at most Z^{7/3} eventually, with \eps fixed. The global density estimate of [9, Lemma 3.3] applies: the state is normalized and antisymmetric and n\le3Z, so its ordinary density \rho_{A_y} obeys \int\rho_{A_y}^{5/3}\le CZ^{7/3}.

Only packet centers in |x|<2r_0 can contribute to the truncated density defining P_0. The potential of a truncated packet is at most that of the full packet, and radial smearing bounds the latter by K(y-x). The observation tower and Hölder’s inequality give

\E[P_0(y)\mid A_y] \le\int_{|x|<2r_0}\frac{\rho_{A_y}(x)}{|y-x|}\,dx \le CZ^{7/5}r_0^{1/5} =C\eps^{6/5}Z/r_0.

Choose \eps so small that the last coefficient is less than 0.05. This contradicts the event definition. Hence \Prob(A_y)\le r_0^{40}.

The minimum packet width is c_1r_0^{1+w}. Integrating |y-z|^{-2} against each bounded packet yields

\norm{\nabla P_0}_\infty\le CZr_0^{-2-2w}.

A spatial net of spacing at most r_0^2 in the annulus has O(r_0^{-3}) points. Its union failure probability is O(r_0^{37}), and its interpolation error divided by Z/r_0 is O(r_0^{1-2w}). This proves Equation (4.5), with the weaker exponent stated there. The good event is measurable because P_0 is continuous in space.

Let G_0 be this good event and define

\mu^{\mathrm{in}}=\ind_{G_0}\ind_{\{d<r_0\}}\mu_0, \qquad p_0=\ind_{G_0^c}\ind_{\{d<r_0\}}\mu_0.

On d<2r_0 consider the branch

v=V-K*\mu^{\mathrm{in}}-0.7Z/r_0 +C_3(Z/r_0)^{3/2}d^2.

Fix C_3 so that 6C_3\ge4\pi k\,2^{3/2} and decrease \eps if necessary so that 4C_3\eps^{3/2}\le0.05. Since Zr_0^3=\eps^3, the quadratic term is at most 0.05Z/r_0 on this ball. On r_0\le d<2r_0 we have v\le2Z/r_0, and therefore

\Delta v=-4\pi\nu+4\pi\mu^{\mathrm{in}} +6C_3(Z/r_0)^{3/2}, \qquad 6C_3(Z/r_0)^{3/2}\ge f(v).

On the lower overlap r_0\le d<1.06r_0,

v\ge(1/1.06-0.1-0.7)Z/r_0>0.14Z/r_0;

on G_0^c the same bound follows with the 0.1 term omitted. On 1.9r_0<d<2r_0,

v\le(1/1.9-0.7+0.05)Z/r_0<0.

Fix B satisfying the subsolution condition above and 0<B\le0.1\eps^3. Define u_0 on an open cover by

u_0= \begin{cases} v,&d<1.06r_0,\\ \max(v,b_{r_0}),&r_0<d<2r_0,\\ b_{r_0},&d>1.9r_0. \end{cases}

The definitions agree on overlaps. Near d=r_0 the branch v alone is active and supplies both required source inequalities. Elsewhere the weak maximum rule proves Equation (4.3). The exterior cap holds for C_{\mathrm{inv}}\ge\max(B,32\eps^3), and

\E\int p_0\le n\Prob(G_0^c)\le Cr_0^{32}.

Choice of the remaining constants. Increase C_{\mathrm{inv}} to exceed the universal cap C_{\mathrm{cap}} in Proposition 3.2. Choose

0<\lambda_2<\lambda_1<\gamma/2, \qquad M>2,\qquad C_{\mathrm{inv}}M^{-4}<\lambda_2.

The constants \lambda_1,\lambda_2 are barrier shifts, distinct from the electron price \lambda=s^{-4}. Fix 0<h_l<B/4 and h_h>C_{\mathrm{inv}}, and then choose e_0,\xi>0 so small that

\begin{gathered} 2e_0(2M)^4<B/4,\qquad 16\xi+2e_0<\lambda_1-\lambda_2,\\ \xi<\min(\lambda_2,h_l/16). \end{gathered} \tag{4.6}

All these constants are now fixed. The simultaneous comparison Proposition 3.2 applies with exactly these parameters along the regime under consideration.

One outward step. Suppose the invariant holds at r=r_j, where j<J_*, and set R=2r and u=u_j. On the good event of Proposition 3.2 for the band r\le d\le4Mr, use

v_1=u-\lambda_1R^{-4},\qquad v_2=H'_j-\lambda_2R^{-4}.

The two branches have complementary roles. On the gained annulus r\le d<R, the old reaction must supply the actual density, so a retained v_1 must satisfy f(u)\ge4\pi\mu_j. Outside R, the field branch already has Laplacian 4\pi\mu_j, which must instead dominate f(v_2). The opposite inverse implications in Equation (3.6), together with the unequal shifts, give these two inequalities on the neighborhoods used below. On bad data omit v_2. Define \widetilde u by

\begin{array}{c|c} \text{region}&\widetilde u\\ \hline d<1.08R&\max(v_1,v_2)\\ 1.04R<d<2MR&\max(v_1,v_2,b_R)\\ d>MR&b_R \end{array} \tag{4.7}

with the same omission on bad data, and set

\widetilde p=p_j+\ind_{\{\mathrm{bad}\}}\ind_{\{r\le d<R\}}\mu_j. \tag{4.8}

Figure 1 shows the overlapping regions in Equation (4.7) and the source-gain annulus r\le d<R. On the lower overlap, Equation (4.2) gives v_1\ge b_r-\lambda_1R^{-4}>b_R. On the upper overlap, the caps and C_{\mathrm{inv}}M^{-4}<\lambda_2 put both shifted branches below b_R. Thus the definitions agree. They give b_R\le\widetilde u\le C_{\mathrm{inv}}d^{-4} on d\ge R and \widetilde u=b_R on d>MR; for R\le d<1.08R the lower bound already follows from v_1.

Figure 1: The overlapping definitions in one continuation step from r to R=2r. The shifted branches are v_1=u_j-\lambda_1R^{-4} and v_2=H'_j-\lambda_2R^{-4}; the second branch is omitted on bad data. The source term changes on the shaded annulus r\le d<R. The barrier gap makes the first two definitions agree on 1.04R<d<1.08R, and the caps make the last two agree on MR<d<2MR.

It remains to prove the weak inequality before averaging. We do so on open neighborhoods, to avoid differentiating across the sets where the maximizing branch changes. At a point in one of the open regions in Equation (4.7), retain the candidates whose value is within e_0R^{-4} of the maximum there. By continuity and finiteness, there is a neighborhood on which every discarded candidate remains strictly below a fixed retained maximizer and every retained candidate v satisfies

\widetilde u-v<2e_0R^{-4}. \tag{4.9}

The maximum of the retained family is still \widetilde u throughout this neighborhood. At the origin use the continuous offsets from V to make the same selection.

Every retained branch satisfies the common inequality

\Delta v\ge-4\pi\nu+4\pi\ind_{\{d<R\}}\mu_j -4\pi\widetilde p+\ind_{\{d\ge R\}}f(v) \tag{4.10}

on this whole neighborhood. For v_1, its old inequality suffices on d<r, and on d\ge R use f(u)\ge f(v_1). The only new source is on r\le d<R. Bad data there are paid for by Equation (4.8). On good data v_2 is a candidate, so Equation (4.9) gives

H'_j\le u-(\lambda_1-\lambda_2-2e_0)R^{-4}.

Moreover h_l<7B/8\le d^4u\le C_{\mathrm{inv}}<h_h. If 4\pi\mu_j>f(u), the high implication of Equation (3.6), at height h=d^4u, would give

H'_j\ge u-\xi d^{-4}\ge u-16\xi R^{-4},

contrary to Equation (4.6). Hence 4\pi\mu_j\le f(u), which supplies the required new density.

For v_2 its exact identity \Delta v_2=-4\pi\nu+4\pi\mu_j suffices on d<R. At a remaining point where it is retained, the lower splice or the included barrier gives \widetilde u\ge b_R and d\le2MR. Consequently

d^4v_2\ge\frac{7B}{8}-2e_0(2M)^4>\frac{5B}{8}>h_l, \qquad d^4v_2\le C_{\mathrm{cap}}<h_h.

If 4\pi\mu_j<f(v_2), the low implication of Equation (3.6) would imply

H'_j\le v_2+\xi d^{-4}\le v_2+\xi R^{-4} <v_2+\lambda_2R^{-4}=H'_j,

a contradiction. Thus 4\pi\mu_j\ge f(v_2) there. The branch b_R occurs only outside R and satisfies Equation (4.10) by its subsolution property.

These comparisons concern zero-order densities almost everywhere on the same open neighborhood, including when it crosses d=R. The common reaction is F(y,t)=\ind_{\{d\ge R\}}f(t). It meets the weak maximum rule’s hypotheses; near zero the common V singularity cancels and the reaction vanishes. The rule therefore proves Equation (4.10) for \widetilde u locally. A partition of unity proves it globally.

Forgetting one observation. Define

u_{j+1}=V+\E[\widetilde u-V\mid\mathcal F_{j+1}], \qquad p_{j+1}=\E[\widetilde p\mid\mathcal F_{j+1}].

We justify the conditional integration of the weak inequality. For a fixed system the positive minimum packet width gives deterministic bounds for \mu_j, K*\mu_j, and its first derivatives. The initial truncated potential has the same bounds. Thus the initial offsets have deterministic local Lipschitz bounds; subtracting constants, taking finite maxima, and gluing on the fixed open cover preserve such bounds. Where b_R is used, its offset from V is smooth and separated from the origin. The errors remain bounded densities supported in deterministic balls. Conditional integration preserves these bounds. All fields and flags are jointly measurable; the spatial supremum defining the initial flag can be tested on a countable dense set. Fubini’s theorem therefore permits conditional integration against each smooth compactly supported test. A countable dense family of nonnegative tests, followed by local approximation, supplies simultaneous almost-sure weak inequalities for all tests.

The conditional tower gives \mu_{j+1} as the new inner density, and convexity gives

\E[f(\widetilde u)\mid\mathcal F_{j+1}] \ge f\bigl(V+\E[\widetilde u-V\mid\mathcal F_{j+1}]\bigr).

This proves the first line of Equation (4.3) at R. The deterministic lower and upper bounds, the equality beyond MR, and the error support also pass to the conditional average.

Total error. For r\le |y|<2r, every master packet contributing to \mu_j(y) has center in a fixed annulus comparable to r and width comparable to r^{1+w}. Conditional Jensen, the packet bound, and Equations (2.6) and (2.8) imply

\norm{\mu_j(y)}_{L^2(\Prob)} \le Cr^{-3-3w}\bigl(r^{-3}+\sqrt{D_0r}\bigr) \le Cr^{-6-3w},

since r\le s and D_0\le Cs^{-7}. The bad band event has probability at most Cr^{25}. Cauchy–Schwarz in the data and integration over the gain annulus therefore give

\E\int\ind_{\{\mathrm{bad}\}}\ind_{\{r\le d<R\}}\mu_j \le Cr^{25/2+3-6-3w}=Cr^{19/2-3w}.

The sum over the geometric sequence of scales is at most Cs^{19/2-3w}. Conditional averaging preserves expected total mass. Together with the initial error estimate this proves Equation (4.4) and completes the induction.

5 The limiting field and its charge

We now prove the charge and profile assertions of Theorem 1.2; Proposition 6.2 will identify the energy coefficient. The barrier is available at every intermediate observation scale, before all observations are forgotten. This lets us select conditional fields which satisfy both the local Thomas–Fermi equation and the small-error barrier.

5.1 Selecting conditional data

Take an arbitrary sequence in Equation (2.1), with an arbitrary minimizing index n in each system. By Equation (2.8), after passing to a subsequence we may suppose

q_s:=s^3(Z-n)\longrightarrow q_*.

Choose integers l\to\infty sufficiently slowly and a scale j<J_* such that

\frac1{2l}\le a_*:=\frac{r_j}{s}\le\frac1l. \tag{5.1}

This is possible because r_0/s\to0 and the radii are dyadic. In addition to the fixed parameters used in the barrier construction, apply Proposition 3.2 at this scale with M=l^2, a fixed upper height greater than C_{\mathrm{cap}}+1, and lower height and tolerance sufficiently small in terms of l. On its good event,

\left|\mu_j(y)-k\bigl(H'_j(y)_+\bigr)^{3/2}\right| \le l^{-8}|y|^{-6} \qquad(r_j\le|y|\le ls). \tag{5.2}

Indeed, let u=|y|^4H'_j(y) and v=(|y|^6\mu_j(y)/k)^{2/3}. The cap on u excludes v at or above the upper height: applying the high implication at heights approaching that endpoint would contradict the cap. Above the lower endpoint, the two implications at heights approaching v squeeze u to within the chosen tolerance of v. At or below the lower endpoint they bound u above by that endpoint plus the tolerance. Thus |u_+-v|\le h_l+\xi, with both u_+ and v in [0,h_h+1]; this uses no lower bound on u. Uniform continuity of t\mapsto t^{3/2} on that interval proves the assertion after choosing h_l and \xi sufficiently small. The spatial range is covered because 4Mr_j\ge2ls.

For each fixed l these are fixed parameters of Proposition 3.2; its thresholds hold eventually and its exceptional probability tends to zero. A slow diagonal choice therefore makes Equation (5.2) hold outside a set of probability tending to zero while also ensuring Equation (5.1).

We can select data on which, in addition,

\int p_j\le1, \qquad s^3\int_{|y|>2R_0s}\mu_j(y)\,dy\le\eta_s, \qquad\eta_s\longrightarrow0. \tag{5.3}

The first excluded probability tends to zero by Equation (4.4). For the second, a master packet centered in |x|\le R_0s is contained in |y|\le2R_0s for all sufficiently far systems. The conditional tower and Equation (2.10) show that the expectation of its left side tends to zero, uniformly in j. Markov’s inequality supplies a deterministic threshold \eta_s\to0 with excluded probability tending to zero. These two events and the good comparison event have positive joint probability. Choose a point in their intersection where all the conditional identities and barrier inequalities hold. Only this finite-system selection is needed; every selected density still has total mass exactly n.

5.2 Compactness and the exterior boundary condition

On the selected data, suppress the sequence index and put

F_s(x)=s^4\bigl(V-K*\mu_j\bigr)(sx), \qquad \rho_s(x)=s^6\mu_j(sx).

Then

\Delta F_s=-4\pi Zs^3\delta_0+4\pi\rho_s, \qquad s^4H'_j(sx)=F_s(x)-1.

The total rescaled electron mass need not be bounded. We instead control the screened field through its spherical mean. Newton’s averaging identity and \int\mu_j=n give

\overline F_s(d):=\frac1{4\pi}\int_{\mathbb S^2}F_s(d\omega)\,d\omega =\frac{q_s}{d} +\int_{|x|>d}\left(\frac1d-\frac1{|x|}\right)\rho_s(x)\,dx. \tag{5.4}

In particular \overline F_s(d)\ge q_s/d.

On every compact annulus, Proposition 3.2 gives the uniform pointwise upper bound F_s(x)\le1+C_{\mathrm{cap}}|x|^{-4} for sufficiently far systems. Together with Equation (5.4) and boundedness of q_s, this bounds F_s in local L^1 away from zero: integrate |F_s|=2(F_s)_+-F_s first over spheres and then over radii. Equation (5.2) also bounds \rho_s uniformly on these annuli.

For completeness, choose a ball whose closure avoids the origin, and add to F_s the Coulomb potential of \rho_s restricted to a slightly larger ball. The sum is harmonic on the larger ball. The added potential and its gradient are uniformly bounded by the integrals of |x-y|^{-1} and |x-y|^{-2} against a bounded density. Interior harmonic estimates, using the local L^1 bound, give uniform bounds and equicontinuity on the smaller ball. A diagonal Arzelà–Ascoli argument now gives a subsequence converging locally uniformly on \R^3\setminus\{0\} to a field F_\infty. The scaled error in Equation (5.2) tends to zero locally uniformly, so the densities converge there to k((F_\infty-1)_+)^{3/2}. Hence

\Delta F_\infty=4\pi k\bigl((F_\infty-1)_+\bigr)^{3/2}, \qquad F_\infty(x)\le1+C_{\mathrm{cap}}|x|^{-4}. \tag{5.5}

The equation holds classically off zero. For example, bounded local sources first give local Hölder regularity of the field; the reaction is then locally Hölder, and interior Poisson regularity gives the asserted conclusion.

The selected tail bound says precisely

\int_{|x|>2R_0}\rho_s(x)\,dx\longrightarrow0.

Local uniform density convergence therefore makes F_\infty harmonic on |x|>2R_0. For d>2R_0, the last term of Equation (5.4) is nonnegative and at most d^{-1} times this tail mass. Consequently

\overline F_\infty(d)=q_*/d\qquad(d>2R_0). \tag{5.6}

These facts imply the uniform boundary condition

F_\infty(x)\longrightarrow0\qquad(|x|\to\infty). \tag{5.7}

Here no positivity has yet been assumed. On large annuli rescaled to a fixed annulus, the upper cap bounds the positive part, and Equation (5.6) bounds the integral of the negative part. Interior harmonic estimates thus give a uniform absolute bound for F_\infty throughout the exterior. Given any sequence R_i\to\infty, its dilates F_\infty(R_i x) have a subsequence converging locally on punctured space to a bounded harmonic function, with the same absolute bound on every punctured compact set. Its singularity at zero is removable, and Liouville’s theorem makes it constant. Its spherical mean is zero by Equation (5.6), so the constant is zero. If Equation (5.7) failed, dilating at a sequence of offending radii and taking a convergent subsequence of the corresponding unit directions would contradict this conclusion. This proves uniform decay.

5.3 Transferring the positive barrier

We claim that

F_\infty(x)\ge B|x|^{-4}\qquad(x\ne0). \tag{5.8}

The field in this assertion is the field without the subtracted price. This distinction permits the reaction comparison below.

Fix an outer radius S>0 and write U_s(x)=s^4u_j(sx). Inside a_*, the distributional inequality for U_s and the equation for F_s contain the same point-nucleus and density \rho_s terms; the inequality also contains the rescaled error from p_j. Outside a_*, Equation (5.2) gives, once l>S,

\rho_s(x)\le k\bigl((F_s(x)-1)_+\bigr)^{3/2} +l^{-8}|x|^{-6}.

Define the nonnegative correction potential

L_s=K*\left(s^6p_j(s\,\cdot) +l^{-8}|\cdot|^{-6}\ind_{\{a_*\le|\cdot|\le S\}}\right). \tag{5.9}

Scaling Equation (4.3), subtracting the equation for F_s, and using \Delta K=-4\pi\delta_0 gives on B(0,S)

\Delta(U_s-F_s-L_s) \ge\ind_{\{|x|\ge a_*\}}\bigl[f(U_s)-f(F_s-1)\bigr]. \tag{5.10}

In particular, subtracting L_s cancels both the accumulated source error and the approximation error with the required sign.

Choose any

c>\left(C_{\mathrm{inv}}S^{-4} -\min_{|x|=S}F_\infty(x)\right)_+.

For sufficiently far systems, local uniform convergence on this sphere, the upper bound for U_s, and L_s\ge0 give U_s-F_s-L_s\le c on the boundary. The same inequality holds throughout the ball. Indeed, test Equation (5.10) with (U_s-F_s-L_s-c)_+. On its positive set, U_s>F_s+L_s+c>F_s-1, so the reaction difference is nonnegative. The test yields

\int_{B(0,S)}\left|\nabla(U_s-F_s-L_s-c)_+\right|^2\le0.

It is legitimate on the full ball: the nuclear singularities in U_s-F_s cancel, the remaining offsets are continuous and locally H^1, and the correction is the potential of a bounded compactly supported density for each fixed system. After cancellation all right-hand sides are locally bounded, including near zero, because the reaction term vanishes on |x|<a_*. Approximation therefore allows the compactly supported nonnegative H^1 test.

For each fixed x\ne0, L_s(x)\to0. The first density in Equation (5.9) has mass at most s^3 by Equation (5.3) and is supported in |x|\le a_*. The second has total mass at most

C l^{-8}a_*^{-3}\le C l^{-5},

by Equation (5.1); its density near a fixed nonzero evaluation point is O_x(l^{-8}). Splitting its potential integral into a small ball around that point and its complement proves the claim. Finally, for fixed 0<|x|<S and sufficiently far systems,

U_s(x)\ge B|x|^{-4}\left(1-\frac{a_*}{8|x|}\right).

Pass to the limit in U_s\le F_s+L_s+c, then decrease c to its permitted endpoint. Letting S\to\infty and using Equation (5.7) proves Equation (5.8).

5.4 The singular profile and uniqueness

The dilation argument below is a direct form of the Sommerfeld comparison principle. The homogeneous zero-price profiles are covered by [13, Lemma 4.4 and Remark 4.5], including nonspherical fields. Here dilation removes the unit price near the singularity; a separate comparison then proves uniqueness for the priced equation.

Lemma 5.1 (Unique decaying singular profile). There is at most one classical solution F of

\Delta F=4\pi k\bigl((F-1)_+\bigr)^{3/2} \quad\text{on }\R^3\setminus\{0\}

which tends uniformly to zero at infinity and satisfies c|x|^{-4}\le F(x)\le C|x|^{-4} near zero for some c,C>0. Every such solution has the uniform singular asymptotic

|x|^4F(x)\longrightarrow A_{\mathrm S}:=\left(\frac{12}{4\pi k}\right)^2 \qquad(|x|\downarrow0). \tag{5.11}

If a solution exists, it is radial.

Proof. Let a and b be the lower and upper limits of |x|^4F(x) at zero; the hypotheses give 0<a\le b<\infty. Choose points approaching the upper limit and put t equal to their radii. The dilates u_t(x)=t^4F(tx) satisfy

\Delta u_t=4\pi k\bigl((u_t-t^4)_+\bigr)^{3/2}.

They are bounded above and below by positive multiples of |x|^{-4} on compact annuli. The local potential and harmonic compactness argument used above supplies a subsequential classical limit u with \Delta u=4\pi k u^{3/2}. The definition of b gives u(x)\le b|x|^{-4} for every x\ne0. After taking a subsequence of the unit directions, equality holds at a unit point. The difference u-b|x|^{-4} has a local maximum there, so

4\pi k b^{3/2}\le12b.

The analogous dilation at points approaching the lower limit touches a|x|^{-4} from above at a unit point and gives 4\pi k a^{3/2}\ge12a. Since both constants are positive,

b\le\left(\frac{12}{4\pi k}\right)^2\le a.

This proves Equation (5.11). The contact argument does not assume radiality.

Let F_1,F_2 be two such solutions. For \alpha>1 and \delta>0, the function G=\alpha F_1+\delta is an upper comparison function:

\Delta G=\alpha\,4\pi k\bigl((F_1-1)_+\bigr)^{3/2} \le4\pi k\bigl((G-1)_+\bigr)^{3/2}.

If F_1\le1 the inequality is immediate; otherwise use G-1\ge\alpha(F_1-1) and \alpha^{3/2}\ge\alpha. The common asymptotic coefficient makes G dominate F_2 on all sufficiently small spheres. Uniform decay and \delta>0 give domination on all sufficiently large spheres. On the intervening annulus, testing with (F_2-G)_+ and using the nondecreasing reaction proves F_2\le G. Thus this inequality holds everywhere. Let \delta\downarrow0 and \alpha\downarrow1, and interchange the two solutions to obtain equality. Rotations preserve the equation and both boundary conditions, so uniqueness also gives radiality.

The charge assertion of Theorem 1.2. The field F_\infty constructed above satisfies the hypotheses of Lemma 5.1, by Equations (5.5), (5.7) and (5.8). In particular a solution exists, is unique, and is radial. Its exterior mean determines q_* uniquely by Equation (5.6). Moreover, at any fixed d>2R_0,

\frac{q_*}{d}=\overline F_\infty(d)\ge Bd^{-4}>0.

Denote this uniquely determined positive number by q. The reaction density vanishes beyond 2R_0, and radiality together with Equation (5.6) gives F_\infty(x)=q/|x| there.

Every sequence of systems and every choice of minimizing indices has bounded scaled deficits by Equation (2.8). From any subsequence on which these deficits converge, the preceding construction produces the same unique profile and hence the same limit q. Therefore all scaled deficits converge to q:

s^3(Z-n)\longrightarrow q>0 \qquad\text{along }\text{Equation (2.1)}.

The argument allowed an arbitrary minimizing index at every stage, as required. The remaining coefficient identity in Theorem 1.2 is proved in Proposition 6.2.

6 Fixed particle numbers and the Thomas–Fermi coefficient

We first recover fixed-sector energy differences from the priced deficit proved in Section 5. This step uses monotonicity of the sector energies, without requiring convexity or requiring every sector to minimize at some price. The priced minimum is concave in the price, and its minimizing sectors bound its secant slopes even when the minimizing sector changes. Integrating the deficit law therefore determines the energy at those sectors; monotonicity then brackets the desired particle number. We identify the coefficient by the corresponding Thomas–Fermi calculation.

6.1 Integrating the price and bracketing the sector

Proposition 6.1. Let q be the deficit coefficient in Theorem 1.2. For every sequence of integers Z>m\ge1 such that m\to\infty and Z/m\to\infty,

\frac{E_Z(Z-m)-E_Z(Z)}{m^{7/3}} \longrightarrow\frac37q^{-4/3}. \tag{6.1}

Proof. Fix such a sequence. At each fixed t>0, choose any index n_t minimizing E_n+tm^{4/3}n, and put

d_{Z,m}(t)=\frac{Z-n_t}{m},\qquad G_{Z,m}(t)=m^{-7/3} \bigl[P(tm^{4/3})-tm^{4/3}Z-E_Z(Z)\bigr].

The choice s=t^{-1/4}m^{-1/3} satisfies Equation (2.1), since Zs^3=t^{-3/4}Z/m\to\infty. The deficit assertion of Theorem 1.2 therefore gives

d_{Z,m}(t)\longrightarrow qt^{3/4} \qquad\text{for every fixed }t>0, \tag{6.2}

for every choice of the minimizing indices.

For 0<v<t, the minimizers at the two endpoint prices give

-d_{Z,m}(t)\le \frac{G_{Z,m}(t)-G_{Z,m}(v)}{t-v} \le-d_{Z,m}(v). \tag{6.3}

Indeed, evaluating the objective at n_v gives the upper inequality, and evaluating the objective at n_t at price v gives the lower one. These inequalities do not require differentiability at a price with more than one minimizing sector.

Take a fixed partition v=t_0<t_1<\cdots<t_r=t. Summing Equation (6.3) bounds G_{Z,m}(t)-G_{Z,m}(v) by the two endpoint Riemann sums for the negative deficits. First use Equation (6.2) at the finitely many partition points, and then refine the partition. Since qt^{3/4} is continuous, this proves

G_{Z,m}(t)-G_{Z,m}(v) \longrightarrow-\frac47q\bigl(t^{7/4}-v^{7/4}\bigr). \tag{6.4}

The behavior at zero price fixes the integration constant. The neutral sector is a competitor, whereas E_{n_v}\ge E\ge E_Z(Z)-C by Equation (2.2); hence

-Cm^{-7/3}-v\,d_{Z,m}(v)\le G_{Z,m}(v)\le0. \tag{6.5}

For every fixed v>0 this gives \limsup|G_{Z,m}(v)|\le qv^{7/4}. Combining it with Equation (6.4) and then sending v\downarrow0 yields

G_{Z,m}(t)\longrightarrow-\frac47qt^{7/4},\qquad \frac{E_{n_t}-E_Z(Z)}{m^{7/3}} =G_{Z,m}(t)+t\,d_{Z,m}(t) \longrightarrow\frac37qt^{7/4}. \tag{6.6}

Thus no assertion about the convergence of the priced minimizers as t\downarrow0 was needed.

Choose fixed prices

0<t_-<q^{-4/3}<t_+.

By Equation (6.2), their deficits are eventually smaller and larger than m, respectively. Thus n_{t_-}>Z-m>n_{t_+}. Monotonicity of the sector energies gives

E_{n_{t_-}}-E_Z(Z) \le E_Z(Z-m)-E_Z(Z) \le E_{n_{t_+}}-E_Z(Z).

Apply Equation (6.6) and let both prices approach q^{-4/3}. The two bounds converge to \frac37q(q^{-4/3})^{7/4}=\frac37q^{-4/3}, proving Equation (6.1).

6.2 The same charge in Thomas–Fermi theory

The classical weak-ionization law was established by Bénilan and Brezis [2, Section 6, Corollary 5], following the bounds and chemical-potential integration argument of Lieb and Simon [7, Theorems IV.11–IV.12]. We give the argument in the present normalization to identify its coefficient with the charge obtained from the conditional quantum limit.

We allow real nuclear charges and real electron masses in this subsection. For clarity, the admissible finite-mass class can be written as

\mathcal X=\{\rho\ge0:\rho\in L^1(\R^3)\cap L^{5/3}(\R^3)\}.

All terms of \mathcal T_Z are finite on this class. For the direct term, interpolation gives \rho\in L^{6/5}, and the Sobolev inequality gives the embedding L^{6/5}\subset(\dot H^1)^* and the finite Coulomb energy. For the nuclear term, use |x|^{-1}\in L^{5/2}_{\mathrm{loc}} near zero and the finite mass away from zero. Thus this is precisely the finite-mass class in the definition of E_Z^{\TF}(M).

Proposition 6.2. With the two-spin coefficient T fixed above,

\lim_{Z\to\infty} \bigl[E_Z^{\TF}(Z-1)-E_Z^{\TF}(Z)\bigr] =\frac37q^{-4/3}. \tag{6.7}

The limit holds through real charges Z>1. Consequently Equation (1.2) holds for every fixed real m>0, with

a_{\TF}=\frac37q^{-4/3}>0.

Proof. We identify the charge in the unit-price Thomas–Fermi problem, then integrate in the price and use the exact density scaling.

Monotonicity in the electron mass. The energy E_Z^{\TF}(M) is nonincreasing in M. To see this without an attainment assumption, truncate any admissible density of mass M_1 to a large ball. The kinetic, nuclear, and direct terms converge to the original ones. If M_2\ge M_1, place the missing mass in a nonnegative smooth packet of diameter proportional to R, centered at distance R^2 from that ball. For a packet of mass a and this spatial scale, its kinetic and direct energies are O(a^{5/3}R^{-2}) and O(a^2R^{-1}). Its nuclear term and its interaction with the fixed truncated density tend to zero as R\to\infty. The mass a stays bounded during this construction. Taking first R\to\infty, then the truncation radius to infinity, and then the original energy down to its infimum proves monotonicity. The same argument shows that imposing mass exactly M or at most M gives the same infimum.

The zero-price minimizer is neutral. Apply [9, Lemmas 7.1 and 7.2] to the single positive point source Z\delta_0. Their unconstrained problem on L^{5/3}\cap(\dot H^1)^* has a unique minimizer \rho_0, with finite mass at most 2Z. Its field \phi_0=V-K*\rho_0 satisfies

\rho_0=k(\phi_0)_+^{3/2},\qquad \Delta\phi_0=-4\pi Z\delta_0+4\pi\rho_0,\qquad c\min\left(\frac Z{|x|},|x|^{-4}\right) \le\phi_0(x)\le C|x|^{-4}. \tag{6.8}

The cited lemmas supply the lower bound, finite mass, and decay at infinity. For completeness, the upper bound is independent of Z: on a ball B(x,R) with R=|x|/2, compare \phi_0 with

v(y)=\frac{C R^4}{(R^2-|y-x|^2)^4}.

For sufficiently large universal C, direct differentiation gives \Delta v\le4\pi k v^{3/2}. The function diverges at the boundary, and the positive-part comparison for \Delta\phi_0=4\pi k\phi_0^{3/2} in this ball gives \phi_0(x)\le CR^{-4}, as asserted.

Uniqueness makes \rho_0 and \phi_0 radial. Newton’s spherical-mean identity and finite mass give

Z-\int\rho_0=\lim_{d\to\infty}d\phi_0(d)=0,

where the last equality follows from Equation (6.8). Therefore \int\rho_0=Z and

E_Z^{\TF}(Z)=\min_{\rho\in\mathcal X}\mathcal T_Z(\rho). \tag{6.9}

There is no discrepancy between the variational classes here: every finite-mass admissible density belongs to the cited Coulomb-dual class, and the cited minimizer has finite mass and finite energy terms, hence belongs to \mathcal X.

The unit-price minimizer. Minimize \mathcal T_Z(\rho)+\int\rho over \mathcal X. Removing density from the region V\le1 cannot increase this functional: the kinetic term, the contribution \int(1-V)\rho there, and all removed direct interactions are nonnegative. We may therefore restrict to the ball B(0,Z). Since V\in L^{5/2}(B(0,Z)), coercivity and weak lower semicontinuity in L^{5/3} give a minimizer, and strict convexity of the kinetic term gives uniqueness. Denote it by \rho_Z and put \phi_Z=V-K*\rho_Z. Nonnegative variations, followed by two-sided multiplicative variations on the positive density, give

\rho_Z=k\bigl((\phi_Z-1)_+\bigr)^{3/2},\qquad \Delta\phi_Z=-4\pi Z\delta_0+4\pi\rho_Z. \tag{6.10}

This holds globally: outside B(0,Z) one has \phi_Z\le V\le1. The minimizer and its field are radial by uniqueness.

The following comparison is the unit-price case of the classical chemical-potential comparison [13, Lemma 5.1]; we include the short maximum-principle proof. The two fields satisfy

\phi_0\le\phi_Z\le\phi_0+1. \tag{6.11}

For the first inequality, on a positive set of \phi_0-\phi_Z-\eta, with \eta>0, the difference of the two reaction terms in Equations (6.8) and (6.10) is nonnegative. Testing with that positive part gives a nonpositive squared-gradient bound and hence a zero test. The test is compactly supported because both potentials tend to zero at infinity. For the second inequality, \phi_0+1 solves the same unit-price equation away from the common point source, and the same comparison applies. At the origin the point singularities cancel; the remaining potentials are continuous and locally H^1, with locally L^{5/3} source densities. Thus the compact tests are justified by H^1 approximation. Let \eta\downarrow0 to obtain Equation (6.11). The continuity and decay used here hold for Coulomb potentials of finite L^1\cap L^{5/3} densities, as also proved in [9, Lemma 7.1].

Write

Q_Z=Z-\int\rho_Z.

By Equation (6.11), \phi_Z\ge0 and \rho_Z\le k\phi_0^{3/2}\le C|x|^{-6}. Newton’s identity reads

\phi_Z(d)=\frac{Q_Z}{d} +\int_{|y|>d}\left(\frac1d-\frac1{|y|}\right)\rho_Z(y)\,dy. \tag{6.12}

Finite mass gives Q_Z=\lim_{d\to\infty}d\phi_Z(d)\ge0. At d=1, the nonnegative second term and Equation (6.11) give Q_Z\le\phi_Z(1)\le C+1. Using the exterior integral of C|y|^{-6} in Equation (6.12), we conclude

0\le\phi_Z(d)\le\frac C d+Cd^{-4}. \tag{6.13}

Choose a fixed sufficiently large R. Then \phi_Z<1 on d>R for every Z, so Equation (6.10) implies \rho_Z=0 there and \phi_Z(d)=Q_Z/d.

Identification of the limiting charge. Let Z\to\infty through real values. On every compact annulus, Equations (6.8) and (6.11) bound \phi_Z above and below, and Equation (6.10) bounds its source. Local Poisson estimates give a locally uniformly convergent subsequence. Its limit \phi_\infty satisfies Equation (5.5) and

c|x|^{-4}\le\phi_\infty(x)\le1+C|x|^{-4}.

The uniform estimate Equation (6.13) gives decay at infinity. By the uniqueness in Lemma 5.1, this is the same field constructed in Section 5. Its exterior charge is q. At any fixed radius beyond both exterior supports, Q_Z=d\phi_Z(d)\to d\phi_\infty(d)=q. Uniqueness of the subsequential limit therefore proves

Q_Z\longrightarrow q\qquad(Z\longrightarrow\infty). \tag{6.14}

The use of real charges is permitted by the arbitrary-positive-point-source hypotheses of [9, Lemmas 7.1 and 7.2].

Other prices and their energies. For t>0, let \rho_{Z,t} minimize \mathcal T_Z(\rho)+t\int\rho, and write Q_Z(t)=Z-\int\rho_{Z,t}. Existence and uniqueness follow as above, now restricting to B(0,Z/t). With b=t^{-1/4}, the transformation

\widetilde\rho(x)=b^6\rho_{Z,t}(bx),\qquad \widetilde\phi(x)=b^4\bigl(V-K*\rho_{Z,t}\bigr)(bx)

gives the unit-price minimizer and field at nuclear charge b^3Z. Indeed, the transformed functional is exactly

\mathcal T_{b^3Z}(\widetilde\rho)+\int\widetilde\rho =b^7\left(\mathcal T_Z(\rho_{Z,t}) +t\int\rho_{Z,t}\right),

and this transformation is a bijection of admissible densities. Its mass is multiplied by b^3, so

Q_Z(t)=t^{3/4}Q_{t^{-3/4}Z} \longrightarrow qt^{3/4} \qquad(t>0\text{ fixed}). \tag{6.15}

Define

\Pi_Z(t)=\min_{\rho\in\mathcal X} \left(\mathcal T_Z(\rho)+t\int\rho\right),\qquad G_Z^{\TF}(t)=\Pi_Z(t)-tZ-E_Z^{\TF}(Z).

The endpoint-minimizer comparisons give, for 0<v<t,

-Q_Z(t)\le \frac{G_Z^{\TF}(t)-G_Z^{\TF}(v)}{t-v} \le-Q_Z(v).

The exact zero-price identity Equation (6.9) gives

-vQ_Z(v)\le G_Z^{\TF}(v)\le0.

Consequently the same fixed-partition integration and then v\downarrow0 argument used in Equations (6.4) and (6.5) gives

G_Z^{\TF}(t)\longrightarrow-\frac47qt^{7/4},\qquad \mathcal T_Z(\rho_{Z,t})-E_Z^{\TF}(Z) \longrightarrow\frac37qt^{7/4}. \tag{6.16}

Each priced minimizer is also a minimizer at its own mass: an improvement at that mass would improve the priced objective. For fixed t_-<q^{-4/3}<t_+, Equation (6.15) places these two masses on opposite sides of Z-1 for all large Z. The mass monotonicity proved above and Equation (6.16), followed by t_-,t_+\to q^{-4/3}, give Equation (6.7).

Every fixed removed mass. For m>0 the density scaling

\rho(x)=m^2\sigma(m^{1/3}x)

multiplies the mass by m and satisfies \mathcal T_Z(\rho)=m^{7/3}\mathcal T_{Z/m}(\sigma). It is a bijection between the corresponding admissible classes. Hence

E_Z^{\TF}(N)=m^{7/3}E_{Z/m}^{\TF}(N/m),\qquad I_m^{\TF}(Z)=m^{7/3}I_1^{\TF}(Z/m). \tag{6.17}

For fixed m>0, the real charge Z/m tends to infinity with Z. Applying Equation (6.7) proves Equation (1.2) and the claimed value of a_{\TF}. This also completes the coefficient assertion of Theorem 1.2.

6.3 The specified order of limits

Completion of the proof of Theorem 1.1. The joint conclusion Equation (1.3) follows from Propositions 6.1 and 6.2. To deduce the iterated limits, suppose first that, along unbounded integers m_j, the normalized inner upper limit exceeds a_{\TF} by a fixed \eta>0. By the definition of a limsup, for each j one may choose an arbitrarily large integer Z_j>m_j, in particular Z_j/m_j\ge j, with

\frac{I_{m_j}(Z_j)}{m_j^{7/3}}>a_{\TF}+\eta/2.

This contradicts Equation (1.3). The same selection applies if these inner upper limits are infinite. Likewise, a normalized inner lower limit less than a_{\TF}-\eta along unbounded m_j allows choosing Z_j/m_j\ge j with normalized energies below a_{\TF}-\eta/2, again a contradiction. Therefore

\limsup_{m\to\infty} \frac{\limsup_{Z\to\infty}I_m(Z)}{m^{7/3}}\le a_{\TF}, \qquad \liminf_{m\to\infty} \frac{\liminf_{Z\to\infty}I_m(Z)}{m^{7/3}}\ge a_{\TF}.

Since the inner lower limit never exceeds the inner upper limit, both outer limits exist and equal a_{\TF}. The construction always chooses Z only after m is fixed; no convergence in Z at a fixed m has been assumed.

References

  1. [1]R. Benguria and Elliott H. Lieb. The most negative ion in the Thomas–Fermi–von Weizsäcker theory of atoms and molecules. Journal of Physics B: Atomic and Molecular Physics, 18(6):1045–1059, 1985. doi:10.1088/0022-3700/18/6/006.
  2. [2]Philippe Bénilan and Haïm Brezis. Nonlinear problems related to the Thomas–Fermi equation. Journal of Evolution Equations, 3:673–770, 2004. https://doi.org/10.1007/s00028-003-0117-8. doi:10.1007/s00028-003-0117-8.
  3. [3]Enrico Fermi. Un metodo statistico per la determinazione di alcune proprietà dell’atomo. Rendiconti dell’Accademia Nazionale dei Lincei, 6:602–607, 1927.
  4. [4]Victor Ivrii. Asymptotics of the ground state energy of heavy molecules and related topics. 2017. arXiv:1210.1132v2. https://arxiv.org/abs/1210.1132v2. arXiv:1210.1132v2.
  5. [5]Elliott H. Lieb. Thomas–Fermi and related theories of atoms and molecules. Reviews of Modern Physics, 53(4):603–641, 1981. Erratum: Reviews of Modern Physics 54 (1982), 311. doi:10.1103/RevModPhys.53.603.
  6. [6]Elliott H. Lieb and Barry Simon. Thomas–Fermi Theory Revisited. Physical Review Letters, 31(11):681–683, 1973. doi:10.1103/PhysRevLett.31.681.
  7. [7]Elliott H. Lieb and Barry Simon. The Thomas–Fermi theory of atoms, molecules and solids. Advances in Mathematics, 23(1):22–116, 1977. https://doi.org/10.1016/0001-8708(77)90108-6. doi:10.1016/0001-8708(77)90108-6.
  8. [8]Elliott H. Lieb and Walter E. Thirring. Bound for the Kinetic Energy of Fermions Which Proves the Stability of Matter. Physical Review Letters, 35(11):687–689, 1975. Erratum: Physical Review Letters 35 (1975), 1116. doi:10.1103/PhysRevLett.35.687.
  9. [9]OpenAI. Uniform excess charge for Coulomb molecules and the outer radius of neutral atoms. OpenAI Math Release preprint PDF, 2026. Reading view on this site: Uniform excess charge for Coulomb molecules and the outer radius of neutral atoms.
  10. [10]Michel Rumin. Balanced distribution-energy inequalities and related entropy bounds. Duke Mathematical Journal, 160(3):567–597, 2011. doi:10.1215/00127094-1444305, arXiv:1008.1674.
  11. [11]Luis A. Seco, Israel M. Sigal, and Jan Philip Solovej. Bound on the ionization energy of large atoms. Communications in Mathematical Physics, 131(2):307–315, 1990. doi:10.1007/BF02161416.
  12. [12]Jan Philip Solovej. Proof of the ionization conjecture in a reduced Hartree–Fock model. Inventiones mathematicae, 104:291–311, 1991. doi:10.1007/BF01245077.
  13. [13]Jan Philip Solovej. The ionization conjecture in Hartree–Fock theory. Annals of Mathematics, 158(2):509–576, 2003. https://doi.org/10.4007/annals.2003.158.509. doi:10.4007/annals.2003.158.509.
  14. [14]Jan Philip Solovej. A new look at Thomas–Fermi theory. Molecular Physics, 114(7–8):1036–1040, 2016. doi:10.1080/00268976.2015.1130273, arXiv:1601.00497.
  15. [15]L. H. Thomas. The calculation of atomic fields. Proceedings of the Cambridge Philosophical Society, 23(5):542–548, 1927. doi:10.1017/S0305004100011683.