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Triangular minimality for planar Coulomb renormalized energy

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Part of family 090: Triangular-lattice optimality, long-range Riesz and Coulomb energies, and spherical logarithmic energy. Read it with its family

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Abstract

We prove the Sandier–Serfaty conjecture: the triangular lattice of covolume one minimizes planar Coulomb renormalized energy over all admissible curl-free fields with a unit uniform background. Combined with Bétermin and Sandier’s asymptotic formula, this also proves the Brauchart–Hardin–Saff conjecture for the linear term of optimal ordered-pair logarithmic energy on the unit two-sphere. The proof uses a direct Voronoi-cell comparison with rigorous interval arithmetic.

1 Introduction

The Coulomb interaction in two dimensions is logarithmic. An infinite configuration of equal point charges against a uniform neutralizing background has an infinite electrostatic energy, even in a bounded region containing a charge. Subtracting the logarithmic self-energy at each charge and then taking energy per unit area gives the renormalized energy studied here. Its proposed minimizer is the triangular lattice.

1.1 The energy and the main results

For R>1, let K_R=[-R,R]^2. Fix smooth cutoffs \chi_R\in C_c^\infty(\R^2) satisfying

0\leq\chi_R\leq1,\qquad \supp\chi_R\subset K_R,\qquad \chi_R=1\text{ on }K_{R-1},\qquad \sup_{R>1}\|\nabla\chi_R\|_\infty<\infty. \tag{1.1}

Let \Lambda\subset\R^2 be locally finite and simple, so every point has multiplicity one, and put \nu_\Lambda=\sum_{p\in\Lambda}\delta_p. The admissible class \mathcal A_1 consists of locally integrable vector fields E such that

\operatorname{div}E=2\pi(\nu_\Lambda-1),\qquad \curl E=0,\qquad \sup_{R>1}\frac{\nu_\Lambda(B_R)}{|B_R|}<\infty, \tag{1.2}

where the equations hold in distributions and B_R is the disk of radius R centered at the origin. These conditions imply E\in L^q_{\mathrm{loc}}(\R^2;\R^2) for every 1\leq q<2: locally subtract the finitely many Coulomb singularities and a smooth field with the prescribed constant divergence; the remaining field has harmonic components. Section 2 supplies the details. Consequently the same class results if local L^q integrability is required for any one, or for all, of these exponents.

For E\in\mathcal A_1 define

\begin{align*} W(E,\chi_R) &=\lim_{\eta\downarrow0}\left[ \frac12\int_{\R^2\setminus\bigcup_{p\in\Lambda}B(p,\eta)} \chi_R|E|^2\dd x +\pi\log\eta\sum_{p\in\Lambda}\chi_R(p)\right],\tag{1.3}\\ W(E)&=\limsup_{R\to\infty}\frac{W(E,\chi_R)}{|K_R|}. \tag{1.4}\end{align*}

The local puncture limit exists and is finite. The outer limsup is initially allowed to take either infinite value. The puncture limit is taken first, and the cutoff layer has the fixed width in (1.1) throughout.

Identify \R^2 with \mathbb C when convenient. The triangular lattice of covolume one is

\Lambda_\triangle =\sqrt{\frac{2}{\sqrt3}} \left(\Z(1,0)+\Z\left(\frac12,\frac{\sqrt3}{2}\right)\right). \tag{1.5}

Let h_\triangle be the mean-zero periodic distributional solution of -\Delta h_\triangle=2\pi(\delta_0-1) on \R^2/\Lambda_\triangle, and set E_\triangle=-\nabla h_\triangle.

Theorem 1.1. For every cutoff family satisfying (1.1) and every field E\in\mathcal A_1,

W(E)\geq W(E_\triangle).

The triangular value is finite, and \inf_{E\in\mathcal A_1}W(E)=W(E_\triangle).

In particular W(E)=-\infty is impossible in this class. The inequality includes fields of energy +\infty. No separation, periodicity, or Voronoi-cell bound is imposed on an arbitrary competitor.

The finite-volume statement used to prove Theorem 1.1 has its own exact normalization. For an integer n\geq2, write T_n=\R^2/(\sqrt n\,\Z^2). Given distinct points a_1,\ldots,a_n\in T_n, let h have mean zero and satisfy -\Delta h=2\pi(\sum_{i=1}^n\delta_{a_i}-1) on T_n. Define

\mathcal W_n(h)=\lim_{\eta\downarrow0} \left[\frac12\int_{T_n\setminus\bigcup_{i=1}^n B(a_i,\eta)} |\nabla h|^2\dd x+\pi n\log\eta\right]. \tag{1.6}

Theorem 1.2. For every integer n\geq2 and every configuration of n distinct points on T_n, the potential in (1.6) satisfies

\mathcal W_n(h)\geq nW(E_\triangle).

This is a lower bound on square tori. It does not assert equality on any particular square torus. Constant harmonic fields increase the energy by n|c|^2/2; the required orthogonality follows by integrating the periodic gradient, as proved in (2.12).

The planar minimum also determines the linear term in optimal logarithmic energy for finitely many points on the sphere.

Corollary 1.3 (Spherical logarithmic energy). Let S^2=\{y\in\R^3:\|y\|=1\} be the unit sphere. For each integer n\ge2, define

E_{\log}(n)=\min_{(y_1,\ldots,y_n)\in(S^2)^n} \left(-\sum_{\substack{1\le i,j\le n\\i\ne j}} \log\|y_i-y_j\|\right),

where the sum is over ordered pairs, \|\cdot\| is the Euclidean norm in \R^3, \log is the natural logarithm, and a collision has energy +\infty. Then, as n\to\infty through the integers,

E_{\log}(n)=\left(\frac12-\log2\right)n^2 -\frac n2\log n+C_{\mathrm{BHS}}n+o(n), \tag{1.7}

where

C_{\mathrm{BHS}} =2\log2+\frac12\log\!\left(\frac23\right) +3\log\!\left(\frac{\sqrt\pi}{\Gamma(1/3)}\right), \tag{1.8}

and \Gamma is Euler’s gamma function.

This proves the d=2 case of the logarithmic-energy conjecture of Brauchart, Hardin, and Saff [4, Conjecture 4]. Bétermin and Sandier had already proved the existence of the linear coefficient and shown that it equals (1.8) precisely when the density-one triangular lattice minimizes their planar renormalized energy [1, Theorem 1.5]. Section 8 checks the normalization and applies that equivalence to Theorem 1.1. The conclusion is an asymptotic value, not a construction of near-optimal point sets or an algorithm for Smale’s seventh problem.

1.2 Context and prior work

The finite-vortex renormalized energy of Bethuel, Brezis, and Hélein [2] is an antecedent of the infinite-system energy considered here. Sandier and Serfaty introduced the planar functional in their analysis of microscopic vortex patterns in the Ginzburg–Landau model. They proved existence of a minimum, approximation of its value by square-periodic fields, and triangular optimality among Bravais lattices [17, Theorems 1 and 2]. Their Conjecture 1 asks whether the triangular value is also the minimum over the full admissible class. Theorem 1.1 resolves this conjecture positively. The current normalization in that paper has one point per area 2\pi/m; our density-one convention corresponds to its background m=2\pi.

The lattice comparison belongs to a longer history. The minimization of convergent Epstein zeta sums at fixed covolume was developed by Rankin [14] and Cassels [5], with an error noted in [6] and a repair supplied by Ennola [8] and simplified by Diananda [7]. Montgomery proved triangular minimality of the lattice theta function for every positive Gaussian parameter [11, Theorem 1]. These are comparisons within the lattice class; the issue here is the lower bound for arbitrary admissible configurations.

For the confining-potential class in their Theorem 2, Sandier and Serfaty show that microscopic limits of finite Coulomb minimizers concentrate on minimizers of the planar renormalized energy [18, Theorem 2]. Its minimum also determines a next-order coefficient for optimal logarithmic energy on the sphere [1, Theorem 1.5]. Petrache and Serfaty prove a conditional implication from universal optimality to minimality for Coulomb and Riesz renormalized energies in their configuration-energy normalization [13, Theorem 2 and Corollary 4]. Their periodic comparison uses tori compatible with the reference lattice, not arbitrary square tori, and their planar conclusion is conditional on the Cohn–Kumar conjecture. The companion universal-optimality theorem supplies the Gaussian comparison used in that implication [12, Theorem 1.1 and Corollary 1.3]. The present proof treats the logarithmic functional directly and uses no universal-optimality result as an input.

Two geometric precedents help explain the finite-torus argument. Screening a point charge by a uniform disk yields a separation argument for planar confined logarithmic minimizers; see Lieb, Rougerie, and Yngvason [10, Lemma 3 and Appendix A]. Voronoi moment inequalities combine sharp cell comparisons with Euler’s bound on the average number of sides, as in Gruber’s proof of a theorem of Fejes Tóth [9]. Affine bounds on cell energies, sharp at the regular hexagon, also appear in the Wasserstein model of Bourne, Peletier, and Theil for cells with at least three sides and mass v\ge1.5\cdot10^{-4} [3, Lemma 12]. Here the cell comparison must arise from a trial potential that is continuous off the sites and has the prescribed logarithmic singularities. Its nonradial correction and the two scalar estimates of Section 5 address that requirement, including sectors whose perpendicular foot lies outside the corresponding edge.

The whole-plane reduction below uses Sandier and Serfaty’s local energy estimates and periodic approximation. The finite-torus argument provides the comparison with the triangular value. Throughout, the conclusion concerns energy per unit area: compact changes to a configuration can preserve this value, so the minimum statement alone does not classify all minimizing configurations.

1.3 How the comparison works

The proof separates a finite-torus comparison from the passage to arbitrary fields. The finite comparison identifies the triangular value. Sandier and Serfaty’s approximation theorem supplies periodic fields approaching the unknown full-plane minimum; it does not identify that minimum.

Section 2 checks the conversion from that approximation theorem to our normalization and fixed-width square cutoffs. The main point is to control the boundary error for an arbitrary field whose energy limsup is bounded above, without assuming separation or density one in advance. Local energy estimates give the needed charge density and boundary-strip bound. Proposition 2.4 then transfers any common lower bound on square tori to every field in \mathcal A_1, including the possible infinite-energy cases.

We next prove the finite comparison. On each square torus the point energy attains a minimum. A screened logarithmic potential and the minimum principle separate the minimizing points, as shown in Section 3. Separation is used only for that minimum; once it is bounded below, every other configuration is bounded below by minimality. This is why the main theorems impose no separation condition on their competitors.

The lifted minimizer has convex Voronoi cells, the regions closer to one site than to any other. Each edge and its incident cell determine a sector joining that edge to the site. Counting incidences on the torus gives at most six sectors per point on average. The comparison is not an estimate of the electrostatic energy of an isolated cell. Instead, we construct a single trial potential H on the torus. Its sector formulas have matching traces and satisfy H=-\log r+O(r^2) near each site. Thus H and the Green potential h have matching logarithmic singularities, while the constant term is normalized to zero in H. Proposition 4.3 gives the exact identity

\mathcal W_n(h) =\sum_S J(S)+\frac12\int_{T_n}|\nabla(h-H)|^2.

Here J(S) is the trial potential’s sector contribution: its linear background-interaction term minus one half of its renormalized Dirichlet integral, as defined in (4.10). The identity cancels the matching logarithmic singularities and retains the nonnegative square exactly.

The construction of H uses radial functions common to every sector. At a shared Voronoi edge its trace depends only on the equal distances to the two neighboring sites; along a ray to a vertex it depends only on the vertex radius. These observations glue the local formulas continuously off the sites and give an H^1 function on every punctured torus. The identity is proved for any compatible flat torus whose area equals its number of sites, not just for square tori. A separate one-site triangular torus supplies six regular sectors; there the chosen potential has exactly the triangular Green gradient, so the square term vanishes.

Section 5 constructs the radial functions from the triangular Green expansion and subtracts fixed multiples of sector area and angle. The desired bound has the form

J(S)\ge K+\lambda A(S)+\mu\theta(S),\qquad K<0.

Areas and angles sum exactly to n and 2\pi n on a square torus. The incidence count then gives n(6K+\lambda+2\pi\mu), and exact calibration on the triangular torus identifies this with nW(E_\triangle).

The perpendicular from a site to a Voronoi edge need not lie on the edge, so one endpoint angle of a sector can be negative. A lower bound for a scalar primitive alone does not control the resulting difference of two primitive values. A second estimate bounds the total negative part of its derivative. Together these estimates handle both ordinary and signed sectors without imposing a regular-polygon hypothesis.

Section 6 proves summable analytic bounds for all omitted lattice modes. Section 7 first verifies the retained finite core and then uses the analytic error bounds to enclose the full functions and their derivatives. Midpoint and interpolation errors cover a compact rectangle between mesh points. At the exact triangular point, analytic stationarity and a positive Hessian bound establish the non-strict minimum; an exact formula handles the unbounded exterior. Section 8 combines these results with the geometry and the whole-plane reduction, then derives Corollary 1.3. Appendix A records two complementary methods: an independent coefficient recurrence and sharper exact tail bounds. They preserve additional quantitative information without adding premises to the main comparison.

2 From square tori to the full plane

This section proves the reduction needed for the full admissible class. A uniform lower bound on finite square tori gives the same lower bound for every field in \mathcal A_1. The argument uses the periodic approximation theorem of Sandier and Serfaty, after checking the normalization and the fixed-width cutoffs in the definition of W.

2.1 Local regularity and the puncture limit

The local integrability convention causes no restriction on the competitors: under the distributional equations, membership in L^1_{\mathrm{loc}} already implies membership in every L^q_{\mathrm{loc}}, 1\le q<2.

Lemma 2.1. Let \Lambda\subset\R^2 be simple and locally finite, and let E\in\mathcal D'(\R^2;\R^2) be a distributional vector field satisfying

\operatorname{div}E=2\pi\Bigl(\sum_{p\in\Lambda}\delta_p-1\Bigr), \qquad \operatorname{curl}E=0.

The field is smooth off \Lambda. Near each p\in\Lambda it has the form

E(x)=\frac{x-p}{|x-p|^2}+F_p(x),\qquad F_p\text{ smooth}. \tag{2.1}

Consequently E has a representative in L^q_{\mathrm{loc}} for every 1\le q<2, and W(E,\xi) exists as a finite real number for every smooth compactly supported \xi.

Proof. Choose a disk about p containing no other charge and subtract

E_p^0(x)=\nabla\log|x-p|-\pi(x-p).

Since \Delta\log|x-p|=2\pi\delta_p, the difference E-E_p^0 has zero divergence and curl as a distribution on the disk. The identities

\Delta V_1=\partial_1\operatorname{div}V- \partial_2\operatorname{curl}V, \qquad \Delta V_2=\partial_2\operatorname{div}V+ \partial_1\operatorname{curl}V

and Weyl’s lemma make both components of this difference smooth. On a disk without charges, use E^0(x)=-\pi x instead. This proves (2.1) and smoothness off the charges. The singular function |x-p|^{-1} is locally in L^q exactly when q<2.

Only finitely many charges meet a fixed compact neighborhood of \operatorname{supp}\xi. Choose disjoint small disks about them. In each disk,

\frac12|E(x)|^2-\frac1{2|x-p|^2}\in L^1.

Moreover \xi(x)-\xi(p)=O(|x-p|), so (\xi(x)-\xi(p))/|x-p|^2 is integrable. The remaining singular integral is \pi\xi(p)\log(\rho/\eta), whose divergence cancels the prescribed \pi\xi(p)\log\eta. The integral outside these disks is finite. Thus the puncture limit exists and is finite.

In particular the only possible infinite values of W(E) arise in the large-square limsup. No puncture limit is interchanged with that limsup below.

2.2 Approximation and local energy estimates

We distinguish the current normalization from the electric-field normalization of \mathcal A_1. For b>0, write \mathcal C_b for currents j\in L^1_{\mathrm{loc}}(\R^2;\R^2) with

\operatorname{div}j=0,\qquad \operatorname{curl}j=\rho-b,\qquad \rho=2\pi\sum_{v\in\Lambda}\delta_v, \qquad \rho(B_s)=O(s^2),

where \Lambda is simple and locally finite. Denote their local puncture functional by \mathsf W(j,\xi); its formula is the same as that of W(E,\xi). Put Q_s=(-s,s)^2.

For such a current, the inverse component rotation F=(j_2,-j_1) satisfies \operatorname{div}F=\rho-b and \operatorname{curl}F=0. In the proof of Lemma 2.1, use the local model \nabla\log|x-p|-(b/2)(x-p) near a charge and -(b/2)x off the charges. This gives the radial singular expansion for F and its rotated expansion for j. Orthogonality preserves the squared norm, so the same finite local puncture conclusion holds for j and every smooth compactly supported cutoff. This local argument uses simplicity and local finiteness, but not the charge-growth bound.

For balls and for Q_s, choose cutoffs 0\le\zeta_{U_s}\le1, compactly supported in U_s, equal to one at distance at least one from its boundary, and with uniformly bounded gradients. Write

\mathsf W_U(j)=\limsup_{s\to\infty} \frac{\mathsf W(j,\zeta_{U_s})}{|U_s|}.

Theorem 1(1),(3),(4) of [17] makes the cutoff choice immaterial within each fixed shape family, gives a common finite minimum

M=\min_{\mathcal C_1}\mathsf W_{\mathrm{ball}} =\min_{\mathcal C_1}\mathsf W_Q\in\R, \tag{2.2}

and provides square-periodic j_k\in\mathcal C_1 with \mathsf W_{\mathrm{ball}}(j_k)\to M. Their square periods have side lengths \sqrt{2\pi n_k} for positive integers n_k. The common minimum does not assert equality of the ball and square values of an arbitrary fixed field. Their conditions (1.4)–(1.5) require increasing bounded open sets with \bigcap_{s>0}\overline U_s=\{0\}, left-continuous volumes, |U_s-U_s|\le C|U_s|, and, for every fixed a\in\R^2,

\frac{|(a+U_s)\mathbin\triangle U_s|}{|U_s|}\longrightarrow0.

They further require constants C and \theta<2 such that

U_s+B_1\subset U_{s+C},\qquad U_{s+1}\subset U_s+B_C,\qquad |U_{s+1}\setminus U_s|=O(s^\theta).

Balls and squares satisfy these conditions with \theta=1 and |U_s-U_s|=4|U_s|.

We also use the following nonsharp consequences of Lemma 4.7 and Proposition 4.9 of [17]. The latter is an application of the mass-displacement method developed for Ginzburg–Landau energies in [16]. In the proof of their Lemma 4.7, Sandier and Serfaty credit the dyadic-shell argument for the local L^r estimate to Struwe [19]; the precise weighted estimate used here is theirs. Let U be bounded and open, \widehat U=U+B_1, and suppose \operatorname{div}j=0 and \operatorname{curl}j=\rho-1 in \widehat U. The number n of simple charges there is finite, and j is locally square-integrable off those charges. For 1<r<2, 0\le\xi\le1 compactly supported in U, and \|\nabla\xi\|_\infty\le C_0, Lemma 4.7 implies

\int_U\xi^{r/2}|j|^r \le C_{r,C_0}(|U|+1)^{1-r/2} \bigl(\mathsf W(j,\xi)_++n\log(2+n)+1\bigr)^{r/2}, \tag{2.3}

where a_+=\max\{a,0\}. For n\ge1, this follows by replacing the energy by its positive part, enlarging the logarithmic count, and absorbing the fixed cutoff bounds into the constant. The statement of Lemma 4.7 and the final display of its proof differ by a factor two on the energy term; this weakening covers either form. If n=0, there is no puncture term and Hölder’s inequality gives directly

\int_U\xi^{r/2}|j|^r \le |U|^{1-r/2}\left(\int_U\xi|j|^2\right)^{r/2} =|U|^{1-r/2}\bigl(2\mathsf W(j,\xi)\bigr)^{r/2},

which also implies (2.3). Proposition 4.9 provides one measure g_U, supported in \widehat U and satisfying g_U\ge-C\,\dd x, such that for every smooth compactly supported \xi in U,

\left|\mathsf W(j,\xi)-\int\xi\,\dd g_U\right| \le C n_\xi\bigl(\log(2+n_\xi)+1\bigr) \|\nabla\xi\|_\infty, \tag{2.4}

where

n_\xi=\#\{v\in\Lambda: B(v,C)\cap\operatorname{supp}\nabla\xi\ne\varnothing\}.

The constants in (2.4) are universal. In particular the same g_U works for two different cutoffs. The local smoothness needed in these results follows as in Lemma 2.1, after rotating the components.

2.3 Scaling and comparison of fixed-width cutoffs

Lemma 2.2. Every E\in\mathcal A_1 satisfies

W(E)\ge 2\pi\left(M-\frac14\log(2\pi)\right). \tag{2.5}

In particular W(E)\ne-\infty.

Proof. The case W(E)=+\infty is immediate. Assume that its limsup is bounded above, allowing provisionally W(E)=-\infty. Set m=2\pi and rotate the vector components by

j=(-E_2,E_1),\qquad j'(y)=m^{-1/2}j(y/\sqrt m),\qquad \xi_t(y)=\chi_{t/\sqrt m}(y/\sqrt m).

Thus j\in\mathcal C_m and j'\in\mathcal C_1; the charges of j' are at \sqrt m\,\Lambda. The cutoff \xi_t is supported in \overline Q_t, equals one on \overline Q_{t-\sqrt m}, and has a uniformly bounded gradient. Changing variables in the punctured integral changes its puncture radius from \eta to \sqrt m\,\eta. Consequently, at each fixed t=\sqrt m R,

W(E,\chi_R)=\mathsf W(j',\xi_t) -\frac\pi2\log m\sum_{v\in\sqrt m\Lambda}\xi_t(v). \tag{2.6}

There is no area factor in this local identity.

The charge-growth hypothesis and the upper bound on the limsup give \mathsf W(j',\xi_t)\le Ct^2 for all sufficiently large t. For any fixed A>0, apply (2.3) to \xi_{t+D} with a fixed D>A+\sqrt m+2, in U=Q_{t+D+1}. There are O(t^2) charges in \widehat U, and this cutoff is one on Q_{t+A}, so

\int_{Q_{t+A}}|j'|^r\le C_{r,A}t^2(\log t)^{r/2}, \qquad 1<r<2. \tag{2.7}

Here are the charge estimates that make the boundary error negligible. Fix A>0. Coarea for y\mapsto\|y\|_\infty and (2.7) with A+2 in place of A give radii

s_+\in(t+A,t+A+1),\qquad s_-\in(t-A-1,t-A)

such that both boundary integrals of |j'|^r are at most Ct^2(\log t)^{r/2}. They may be chosen with no charge on either boundary. Stokes’ theorem, first on the punctured square and then letting the punctures shrink, yields

\rho'(Q_{s_\pm})-|Q_{s_\pm}| =\int_{\partial Q_{s_\pm}}j'\cdot\tau\,\dd\mathcal H^1, \qquad \rho'=2\pi\sum_{v\in\sqrt m\Lambda}\delta_v.

Hölder’s inequality bounds the absolute value by Ct^{1+1/r}(\log t)^{1/2}. Monotonicity of \rho' therefore gives

\begin{align*} \rho'(Q_t)&=|Q_t|+o(t^2),\tag{2.8}\\ \rho'(Q_{t+A}\setminus Q_{t-A}) &\le C_A\bigl(t+t^{1+1/r}(\log t)^{1/2}\bigr) =o(t^2/\log t). \tag{2.9}\end{align*}

The last equality uses r>1. In particular

\sum_v\xi_t(v)=\frac{|Q_t|}{2\pi}+o(t^2). \tag{2.10}

Choose a fixed L>\sqrt m+2 and a standard unit-width cutoff \zeta_{Q_{t-L}}. Both this cutoff and \xi_t are compactly supported in U=Q_{t+1}. Their gradient supports, together with any fixed-radius neighborhoods, lie in a strip of the form appearing in (2.9). Hence each error in (2.4) is o(t^2). Since 0\le\zeta_{Q_{t-L}}\le\xi_t\le1, and their difference is supported in \overline Q_t\setminus Q_{t-L-1},

\int(\xi_t-\zeta_{Q_{t-L}})\,\dd g_U \ge-C\int(\xi_t-\zeta_{Q_{t-L}})\,\dd x\ge-O(t).

Using this one measure for both cutoffs proves

\mathsf W(j',\xi_t) \ge\mathsf W(j',\zeta_{Q_{t-L}})-o(t^2). \tag{2.11}

Every boundary width used here is fixed as t\to\infty.

Divide (2.11) by |Q_t| and take limsups. The ratio |Q_{t-L}|/|Q_t| tends to one, so

\limsup_{t\to\infty}\frac{\mathsf W(j',\xi_t)}{|Q_t|} \ge\mathsf W_Q(j')\ge M.

These inequalities hold in the extended real sense. From (2.6), (2.10), and |Q_t|=m|K_R|, we obtain

W(E)=m\left(\limsup_{t\to\infty} \frac{\mathsf W(j',\xi_t)}{|Q_t|} -\frac14\log m\right).

This proves (2.5) and rules out the provisional case W(E)=-\infty.

2.4 Periodic averaging and the harmonic component

For a periodic field F with one unit logarithmic singularity at each of N charges in a period cell P, define its cell energy by

\mathcal E_P(F)=\lim_{\eta\downarrow0} \left[\frac12\int_{P\setminus\bigcup_v B(v,\eta)}|F|^2\,\dd x +\pi N\log\eta\right].

The integral is interpreted on the flat torus, so disks meeting a chosen cell boundary are identified periodically.

Lemma 2.3. Let F be a periodic admissible electric field or current, with simple charges and period cell P of area A. For either square or ball cutoffs with fixed boundary width and uniformly bounded gradients, its energy per unit area has a limit, equal to \mathcal E_P(F)/A.

Proof. There are finitely many charges on the fixed torus. Choose \rho>0 smaller than its injectivity radius, with the disks about distinct torus charges disjoint, and write on its periodic lift

F_\rho(x)=\frac12|F(x)|^2- \sum_v\frac{\mathbf1_{B(v,\rho)}(x)}{2|x-v|^2}.

By the local expansion in Lemma 2.1, with rotated components for currents, F_\rho is periodic and belongs to L^1(P). For a cutoff \xi the puncture calculation gives

\begin{align*} \mathsf W(F,\xi) &=\int\xi F_\rho\,\dd x+\pi\log\rho\sum_v\xi(v)+\mathcal R_\xi,\\ \mathcal R_\xi &=\sum_v\int_{B(v,\rho)} \frac{\xi(x)-\xi(v)}{2|x-v|^2}\,\dd x.\end{align*}

Here \mathsf W denotes the same local formula for either type of field. A summand in \mathcal R_\xi vanishes unless B(v,\rho) meets \operatorname{supp}\nabla\xi, and each has absolute value at most \pi\rho\|\nabla\xi\|_\infty. For a ball or square of size R there are O(R) such charges, with constants allowed to depend on the fixed periodic field. Thus \mathcal R_\xi=O(R).

The number of period cells meeting any fixed-width boundary strip is also O(R). Integrating the periodic L^1 function F_\rho over the remaining complete cells, and bounding the boundary cells by \|F_\rho\|_{L^1(P)}, shows that

\frac1{|U_R|}\int\xi F_\rho\,\dd x \longrightarrow\frac1A\int_PF_\rho\,\dd x, \qquad \frac1{|U_R|}\sum_v\xi(v)\longrightarrow\frac NA.

The resulting limit is (\int_PF_\rho+\pi N\log\rho)/A=\mathcal E_P(F)/A.

On T_n=\R^2/(\sqrt n\,\Z^2), let h be the mean-zero solution of -\Delta h=2\pi(\sum_{i=1}^n\delta_{v_i}-1) for distinct points v_1,\ldots,v_n, with energy defined by (1.6). The compatibility condition holds because |T_n|=n; the mean-zero solution exists and is unique by the Fourier series for the Laplacian on the torus. Any periodic locally integrable curl-free field E with divergence -\Delta h differs from -\nabla h by a smooth field of zero divergence and curl. Each component is harmonic on the torus, hence constant. Therefore E=-\nabla h+c, with c\in\R^2. As a distributional derivative of a periodic function, \nabla h has integral zero; it is in L^1(T_n) by Lemma 2.1. The cross integral on the punctured torus thus tends to zero, giving the exact identity

\mathcal E_{T_n}(E)=\mathcal W_n(h)+\frac n2|c|^2. \tag{2.12}

Applying the same fixed orthogonal rotation to the fields preserves this energy identity.

Proposition 2.4 (Reduction to square tori). Let C\in\R. Suppose that for every integer n\ge2 and every configuration of n distinct points of T_n, the mean-zero potential in (1.6) satisfies \mathcal W_n(h)\ge nC. Then W(E)\ge C for every E\in\mathcal A_1. In particular, if these finite-torus bounds hold with C=W(E_\triangle), then

\inf_{E\in\mathcal A_1}W(E)=W(E_\triangle).

Proof. Take the square-periodic minimizing sequence j_k\in\mathcal C_1 in (2.2). Integrating its curl on a square period torus shows that the area of that torus is 2\pi N_k, where N_k is its positive integer number of charges. If N_k=1, use twice the square period, which has four charges. Lemma 2.3 shows that this change of period preserves the energy per unit area. We may therefore assume N_k\ge2. We may also align each period square with the coordinate axes: simultaneous rotation of the positions and vector components preserves its cell energy, and the same lemma identifies its energy per unit area.

With m=2\pi, rescale and undo the component rotation:

E_k(x)=\sqrt m\bigl((j_k)_2(\sqrt m x), -(j_k)_1(\sqrt m x)\bigr).

This is an admissible field on T_{N_k}. Changing the puncture radius in its cell gives

\mathcal E_{T_{N_k}}(E_k) =\mathcal E_{P_k}(j_k)-\frac\pi2N_k\log m, \qquad |P_k|=mN_k.

Combining periodic averaging, (2.12), and the assumed torus inequality yields

m\left(\mathsf W_{\mathrm{ball}}(j_k)-\frac14\log m\right) =\frac{\mathcal E_{T_{N_k}}(E_k)}{N_k}\ge C.

Letting k\to\infty gives m(M-\frac14\log m)\ge C. Lemma 2.2 now proves the conclusion for every full-plane competitor, including all possible infinite-energy cases.

For the last assertion, the covolume-one triangular lattice is simple, locally finite, and has quadratic charge growth. Its periodic potential gives an element E_\triangle\in\mathcal A_1, whose finite energy follows from Lemmas 2.1 and 2.3. It supplies the opposite inequality for the infimum.

3 Finite tori and separated minimizing configurations

We first isolate the finite-dimensional problem used in the periodic reduction. Separation will be proved only for its minimizing configurations. This suffices for a lower bound on every configuration.

For an integer n\geq2, put

L=\sqrt n,\qquad T_n=\R^2/(L\Z^2).

The torus has area n. Given distinct points v_1,\ldots,v_n\in T_n, let h be the mean-zero distributional solution of

-\Delta h=2\pi\left(\sum_{i=1}^n\delta_{v_i}-1\right).

We use the energy (1.6). For this square-torus energy, \eta is smaller than the injectivity radius and half the minimum distance between the finitely many points.

3.1 Green representation and existence

Lemma 3.1 (Green representation and existence). Let G_n be the mean-zero Green function on T_n, normalized by

-\Delta G_n=2\pi(\delta_0-1/n), \qquad R_n=\lim_{x\to0}\bigl(G_n(x)+\log|x|\bigr).

For every configuration of n distinct points,

h(x)=\sum_{i=1}^nG_n(x-v_i),\qquad \mathcal W_n(h)=\pi nR_n+ \pi\sum_{i\ne j}G_n(v_i-v_j). \tag{3.1}

The minimum of \mathcal W_n over such configurations is attained at a configuration of distinct points.

Proof. The first identity follows from the equation and the zero-mean normalization. Subtracting the logarithmic singularity and applying local elliptic regularity gives, near v_i,

h(x)=-\log|x-v_i|+a_i+O(|x-v_i|),\qquad a_i=R_n+\sum_{j\ne i}G_n(v_i-v_j).

Let \Omega_\eta=T_n\setminus\bigcup_iB(v_i,\eta). On its hole boundaries the outward normal points towards v_i; therefore

\partial_{\boldsymbol n}h=\frac1\eta+O(1).

Since \Delta h=2\pi on \Omega_\eta, integration by parts gives

\frac12\int_{\Omega_\eta}|\nabla h|^2 =-\pi\int_{\Omega_\eta}h +\frac12\sum_i\int_{\partial B(v_i,\eta)} h\,\partial_{\boldsymbol n}h.

The bulk integral tends to zero because h has mean zero. The i-th boundary integral is 2\pi(-\log\eta+a_i)+o(1). Taking the puncture limit proves (3.1).

The function G_n is bounded below on its punctured torus and tends to +\infty at the origin. Extend the right-hand side of (3.1) to +\infty on configurations with a collision. This gives a lower semicontinuous function on the compact space T_n^n, finite at every configuration of distinct points. A collision cannot be canceled by other pair terms, since all those terms have a common finite lower bound. A minimum therefore exists and has distinct points.

By (2.12), every admissible periodic field with these charges differs from -\nabla h by a constant vector c, which adds n|c|^2/2 to the energy. It therefore suffices to minimize over the mean-zero potentials considered here.

3.2 Separation of minimizers

The argument uses a screened logarithmic potential and the minimum principle. A closely related exclusion argument for minimizing configurations of a planar confined system, with the same single-charge screening radius, appears in Lieb, Rougerie, and Yngvason [10, Lemma 3 and Appendix A]. The following proof treats the torus Green function and its background directly.

Lemma 3.2 (Separation). For every n\geq2, a minimizing configuration in Lemma 3.1 has torus distance at least

r_*=\frac1{\sqrt\pi}

between distinct points. Its full lift to \R^2 has the same minimum-separation bound, including between different period translates of one torus point.

Proof. Fix one point q of a minimizing configuration. The symmetry of G_n, together with (3.1), shows that

\Phi(x)=\sum_{p\ne q}G_n(x-p)

has a global minimum at q. At a fixed point p\ne q, interpret \Phi(p)=+\infty.

The injectivity radius of T_n is \sqrt n/2>r_* for n\geq2. We may therefore define a function on the embedded radius-r_* disk by

\phi(x)= \begin{cases} -\log(|x|/r_*)+\dfrac{\pi}{2}(|x|^2-r_*^2), &0<|x|<r_*,\\[3pt] 0,&|x|\geq r_*. \end{cases}

Its value and radial derivative vanish at r_*, and it is positive inside the disk. Consequently

-\Delta\phi=2\pi(\delta_0-\mathbf1_{B(0,r_*)})

without a boundary measure on the circle. Each such disk has area one.

Set

\Omega=\bigcup_{p\ne q}B(p,r_*),\qquad \Psi=\Phi-\sum_{p\ne q}\phi(\,\cdot-p).

All poles cancel. In particular \Psi\in W^{2,s}(T_n) for every finite s, and \Psi is continuous. On \Omega,

-\Delta\Psi =2\pi\sum_{p\ne q}\mathbf1_{B(p,r_*)} -2\pi\frac{n-1}{n} \geq \frac{2\pi}{n}>0.

Since |\Omega|\leq n-1<n, every component of \Omega has nonempty boundary. Every obstacle vanishes on this boundary, so \Psi=\Phi there.

If q\in\Omega, let D be its component. The strict minimum principle, valid for this continuous W^{2,s} supersolution, gives

\Phi(q)>\Psi(q)> \min_{\partial D}\Psi =\min_{\partial D}\Phi\geq\Phi(q),

a contradiction. No regularity of the union’s boundary is required: the minimum is attained on \overline D, and strict superharmonicity excludes an interior minimum. Hence q\notin\Omega. As q was arbitrary, distinct torus points are separated by r_*.

Distances between lifts of distinct torus points are at least their torus distance. Two different lifts of one point differ by a nonzero vector in L\Z^2, whose length is at least L=\sqrt n>r_*.

4 Voronoi sectors and a glued dual potential

We first record the sector geometry of separated square-torus minimizers. We then prove gluing and duality for compatible periodic Voronoi sectors on any flat torus. This separates the general identity from its square-torus and triangular applications. The construction uses general radial functions; their particular choice and triangular calibration will be given later. Its purpose is to turn a sector lower bound, established by two scalar estimates, into an energy bound for a whole configuration.

The use of polygon inequalities together with an average of at most six sides is familiar from moment methods; see Gruber’s proof of Fejes Tóth’s theorem [9]. A related affine cell bound for a Wasserstein interaction is sharp at the regular hexagon of unit mass; the result of Bourne, Peletier, and Theil [3, arXiv v3, Lemma 12] assumes integer side counts at least three and cell mass v\geq1.5\cdot10^{-4}. Here we must construct a globally admissible singular potential before estimating its sector contributions. The arguments below supply that construction and the incidence count on a torus.

4.1 Counting sectors on the torus

For d>0 and real \alpha,\beta with |\alpha|,|\beta|<\pi/2 and \alpha+\beta>0, define the sector

S(d,\alpha,\beta)= \{(r,\varphi):-\alpha<\varphi<\beta,\ 0<r<d\sec\varphi\}. \tag{4.1}

Its polar axis is the normal from its site toward the supporting edge.

Lemma 4.1 (Periodic Voronoi geometry). Let P\subset\R^2 be the full L\Z^2-periodic lift of n distinct points on T_n, and suppose P has separation at least r_*. Its Voronoi polygons, modulo L\Z^2, have at most 6n face–edge incidences.

Each such incidence determines a sector (4.1) in polar coordinates about its site, with d\geq r_*/2. The sectors in one torus have total area n and total angle 2\pi n. Either endpoint parameter \alpha or \beta is allowed to be negative.

Proof. For p\in P, the Voronoi cell

C_p=\{x:|x-p|\leq|x-q|\text{ for all }q\in P\}

contains the disk of radius r_*/2 about p. Comparison with the four sites p\pm(L,0) and p\pm(0,L) gives

C_p\subset p+[-L/2,L/2]^2.

Local finiteness now implies that C_p is a bounded convex polygon with finitely many sides. There are finitely many polygon, edge, and vertex orbits under the period lattice.

Use maximal positive-length Voronoi edges. Each edge has two face incidences, and each vertex has degree at least three. Indeed a Voronoi vertex has at least three nearest sites; a degenerate vertex with more nearest sites only increases the degree. The quotient is a finite cell decomposition of the torus with F=n open faces. Each open face is a disk: distinct translates of the interior of a lift cell are disjoint. A projected closed face need not be embedded, since its boundary may identify to itself. These identifications are permitted in the cell decomposition.

Let V and E denote its numbers of vertices and edges. Euler’s identity and the degree count give

V-E+n=0,\qquad 3V\leq2E.

Thus E\leq3n, and the number of face–edge incidences is M_0=2E\leq6n. These counts include every occurrence in a face boundary: an edge may be a loop, a face may lie on both sides of an edge, a neighbor may recur, and a vertex may occur several times in one boundary. No generic-position assumption is used.

For an edge of C_p shared with C_q, choose as polar axis the unit vector from p towards q. Its supporting line has distance d=|p-q|/2\geq r_*/2 from p. The angular coordinates of its two endpoints satisfy -\pi/2<\varphi_-<\varphi_+<\pi/2. Write \varphi_-=-\alpha and \varphi_+=\beta. The triangle from p to the edge is exactly (4.1). If the perpendicular foot is outside the edge, one of \alpha,\beta is negative.

The sectors partition each polygon up to their boundary rays. A polygon has angle 2\pi about its interior site. Summing areas and angles over the n quotient faces proves the last assertions.

For reference, the area and angle of (4.1) are

A(S)=\frac12\int_{-\alpha}^{\beta}d^2\sec^2\varphi\,\dd\varphi, \qquad \theta(S)=\alpha+\beta. \tag{4.2}

In particular the sector has positive angle even when one endpoint parameter is negative.

Figure 1: Two possible Voronoi sectors, with the edge normal as angular axis. In the right-hand sector both endpoints are above that axis, so the lower endpoint parameter \alpha is negative even though the sector angle \alpha+\beta is positive.

4.2 Compatible flat-torus data and trace matching

Let \Gamma\subset\R^2 be a rank-two lattice and put \mathbb T=\R^2/\Gamma. Let N\geq1 be an integer, let v_1,\ldots,v_N be distinct points of \mathbb T, and let P be their full \Gamma-periodic lift. Suppose that the Voronoi cells of P are bounded convex polygons with finitely many face–edge incidences modulo \Gamma. Assume that each incidence has the sector form (4.1) and that, for one named constant d_0>0, every sector has d\geq d_0. We call these compatible periodic Voronoi data with lower edge distance d_0. This is conditional geometric data, not a separation assertion about an arbitrary competitor.

The sectors partition the N cells modulo \Gamma, up to their boundary rays. Their total area is |\mathbb T|, and their total angle is 2\pi N: each convex cell has its site in its interior because d_0>0, so its sectors have total angle 2\pi. These facts do not require an incidence bound.

Call a radius \eta>0 admissible if it is smaller than the injectivity radius of \mathbb T and, when N\geq2, smaller than half the minimum torus distance between distinct sites. Thus the torus disks B(v_i,\eta) are embedded and pairwise disjoint; for N=1 there is no pairwise-distance condition. Write

\Omega_\eta=\mathbb T\setminus\bigcup_{i=1}^N B(v_i,\eta).

In puncture limits we may further take \eta<d_0, so every deleted disk lies in its Voronoi cell. This restriction does not change a limit as \eta\downarrow0.

Fix compatible periodic Voronoi data with lower edge distance d_0. Let I be a finite or countable index set, and choose integers k_i\geq6, i\in I; different indices may have the same integer. Suppose that

B\in C^1((0,\infty)),\qquad D_i\in C^1((0,\infty))

satisfy the following assumptions:

B(r)=-\log r+O(r^2),\qquad B'(r)=-1/r+O(r) \quad(r\downarrow0), \tag{4.3}

and, for every T_0>d_0,

\sum_{i\in I}\ \sup_{d_0\leq t\leq T_0} \bigl((1+k_i)|D_i(t)|+t|D_i'(t)|\bigr)<\infty. \tag{4.4}

These are the exact inputs needed in the gluing and duality argument. The later radial construction will verify them directly.

For a sector (4.1), define t(\varphi)=d\sec\varphi and

H(r,\varphi)=B(r)+ \sum_{i\in I}\left(\frac r{t(\varphi)}\right)^{k_i} D_i(t(\varphi)). \tag{4.5}

The same radial functions are used in every sector.

Lemma 4.2 (Gluing and singular normalization). For compatible periodic Voronoi data on \mathbb T with N\geq1 distinct sites and lower edge distance d_0, let I be finite or countable, let k_i\geq6 be integers with repetitions permitted, and let B,D_i\in C^1((0,\infty)) satisfy (4.3)–(4.4). The sector functions (4.5) define a \Gamma-periodic function H that is continuous off the sites and belongs to H^1(\Omega_\eta) for every admissible \eta<d_0. At every site, uniformly in the angular variable,

H=-\log r+O(r^2),\qquad \nabla H=-\frac{e_r}{r}+O(r). \tag{4.6}

The gradient statement is sectorwise, and hence holds for the weak gradient almost everywhere; no agreement of derivatives across sectors is asserted. In particular the constant term in H+\log r is zero.

Proof. Fix the finite collection of lifted polygons needed for one torus. Their vertex radii are bounded by some T_0>d_0. On each closed sector, d_0\leq t\leq T_0, r/t\leq1, and \tan\varphi is bounded. The derivatives of a summand are

\partial_r\left[(r/t)^{k_i}D_i(t)\right] =\frac{k_i}{r}(r/t)^{k_i}D_i(t),

and

\partial_\varphi\left[(r/t)^{k_i}D_i(t)\right] =\tan\varphi\,(r/t)^{k_i} \bigl(tD_i'(t)-k_iD_i(t)\bigr).

Assumption (4.4) therefore gives uniform convergence of the series and its first derivatives on each closed sector away from its site. Derivatives here are sectorwise; derivatives across different sectors need not agree.

On a polygon edge, r=t, so the trace is

B(r)+\sum_iD_i(r).

The two adjacent sites have the same distance to that edge point, and hence give the same trace. On a ray from a site to a vertex at distance r_v, either neighboring sector has t=r_v at its endpoint angle. Both traces along the entire ray are

B(r)+\sum_i(r/r_v)^{k_i}D_i(r_v).

At a multiple vertex all incident sites have the same vertex distance, so the edge traces also coincide there. The recipe is unchanged by period translations.

Thus all traces match. Applying the Sobolev gluing property to the finitely many sectors gives the asserted H^1 regularity off the holes. No matching of normal derivatives is required.

For r\leq d_0/2, the fact that every k_i\geq6, together with (4.4), bounds the correction series by O(r^6) and its gradient by O(r^5). Combining these bounds with (4.3) proves (4.6).

The common notation D_i=b_i-u_i, B=\sum_i u_i is one way to supply these data. In that notation the common edge trace is simply \sum_i b_i(r). The gluing argument itself only uses B and D_i.

4.3 The exact dual identity

Assume now that |\mathbb T|=N. Let h be the mean-zero distributional solution on \mathbb T of

-\Delta h=2\pi\left(\sum_{i=1}^N\delta_{v_i}-1\right). \tag{4.7}

The area condition is exactly the compatibility condition for this equation. With the convention

\Gamma^*=\{k\in\R^2:k\cdot\gamma\in\Z \text{ for every }\gamma\in\Gamma\},

the Fourier mode e^{2\pi i k\cdot x} has eigenvalue 4\pi^2|k|^2 under -\Delta. The constant Fourier coefficient of the right-hand side vanishes. Dividing its coefficient at each nonzero k\in\Gamma^* by 4\pi^2|k|^2, and setting the coefficient at zero to zero, gives a distributional solution. It is unique because the kernel of the Laplacian on the torus consists of constants. Define

\mathcal W_{\mathbb T}(h)=\lim_{\eta\downarrow0} \left[ \frac12\int_{\Omega_\eta}|\nabla h|^2\,\dd x+\pi N\log\eta \right], \tag{4.8}

where the limit is taken through admissible radii. The local calculation in Lemma 2.1, applied in a torus chart, gives the finite puncture limit. When \mathbb T=T_n and N=n, this is exactly \mathcal W_n(h) in (1.6).

For a sector S=S(d,\alpha,\beta), define

\int_S^{\mathrm{ren}}|\nabla H|^2 =\lim_{\eta\downarrow0}\left[ \int_{S\cap\{r>\eta\}}|\nabla H|^2\,\dd x +\theta(S)\log\eta\right]. \tag{4.9}

Lemma 4.2 shows that this limit is finite. Its counterterm uses the positive angle \theta(S), also for a sector with a negative endpoint parameter. Define

J(S)=-2\pi\int_S H\,\dd x -\frac12\int_S^{\mathrm{ren}}|\nabla H|^2. \tag{4.10}

The sectorwise estimates in the proof of Lemma 4.2 also show that these expressions are well defined on any individual sector with d\geq d_0 and the endpoint conditions in (4.1), without first choosing a periodic tiling.

Proposition 4.3 (Dual identity). For compatible periodic Voronoi data on \mathbb T=\R^2/\Gamma with N\geq1 distinct sites, lower edge distance d_0>0, and |\mathbb T|=N, let h be the mean-zero potential (4.7). Let I be finite or countable, let k_i\geq6 be integers with repetitions permitted, and let B,D_i\in C^1((0,\infty)) satisfy (4.3)–(4.4). Let H be the function supplied by Lemma 4.2. Then

\mathcal W_{\mathbb T}(h) =\sum_S J(S)+ \frac12\int_{\mathbb T}|\nabla(h-H)|^2\,\dd x \geq\sum_S J(S). \tag{4.11}

The sum runs over all face–edge incidences in one torus. No incidence bound or square-torus separation hypothesis is imposed.

Proof. Apply Lemma 2.1 in a local chart to -\nabla h. Near each site, h=-\log r+a_i+O(r) and \nabla h=-e_r/r+O(1). Thus both h and H have singular gradient -e_r/r. Their difference has square-integrable gradient. Also (4.6) implies that

I_{\mathrm{ren}}(H)= \lim_{\eta\downarrow0}\left[ \int_{\Omega_\eta}|\nabla H|^2+2\pi N\log\eta\right]

exists. For admissible \eta<d_0, the punctured sectors partition \Omega_\eta up to their boundaries. The sector angles sum to 2\pi N, so I_{\mathrm{ren}}(H) equals the sum of (4.9).

Green’s identity, with h smooth on the punctured torus and H\in H^1(\Omega_\eta), gives

\int_{\Omega_\eta}\nabla h\cdot\nabla H =-2\pi\int_{\Omega_\eta}H +\sum_i\int_{\partial B(v_i,\eta)} H\,\partial_{\boldsymbol n}h.

The outward hole normal gives \partial_{\boldsymbol n}h=1/\eta+O(1). The zero constant term in (4.6) therefore gives

\int_{\Omega_\eta}\nabla h\cdot\nabla H =-2\pi\int_{\mathbb T}H-2\pi N\log\eta+o(1).

Expanding |\nabla(h-H)|^2, inserting this identity, and taking the puncture limit proves

\mathcal W_{\mathbb T}(h) =-2\pi\int_{\mathbb T}H-\frac12I_{\mathrm{ren}}(H) +\frac12\int_{\mathbb T}|\nabla(h-H)|^2.

Partitioning the first two terms into sectors proves (4.11).

If the gradient hypotheses were unchanged but the value expansion were instead H=-\log r+c_i+o(1) at v_i, the right-hand side of the last identity would contain the additional term 2\pi\sum_i c_i. This explains why the zero constant term in the radial construction is part of the normalization.

For a square-torus minimizer, Lemma 4.1 supplies the compatible data with \Gamma=\sqrt n\,\Z^2, N=n, and d_0=d_*=r_*/2=1/(2\sqrt\pi). Its torus has area n, so Proposition 4.3 applies with \mathcal W_{\mathbb T}=\mathcal W_n. The triangular application in the next section supplies its own period and sectors and does not use a square-torus minimizer.

4.4 From scalar estimates to configuration bounds

The two scalar bounds below control ordinary and signed sectors by different arguments. Once they yield an affine lower bound for each sector, the dual identity and the incidence count give the energy bound. We formulate this implication for compatible flat tori first; separation of a square-torus minimizer then removes the geometric hypotheses from the finite-volume comparison.

Lemma 4.4 (Signed endpoint parameters). Let K<0 and d_0>0. For each d\geq d_0, let G(d,\cdot) be an even locally integrable real function on \R, and put

g_d(x)=\int_0^xG(d,s)\,\dd s.

Suppose that, for every d\geq d_0,

2g_d(x)\geq K\quad(x\geq0),\qquad \int_0^\infty\max\{0,-G(d,s)\}\,\dd s\leq-K. \tag{4.12}

Then, for every d\geq d_0 and every pair \alpha,\beta with |\alpha|,|\beta|<\pi/2 and \alpha+\beta>0,

g_d(d\tan\alpha)+g_d(d\tan\beta)\geq K. \tag{4.13}

Proof. Evenness of G(d,\cdot) makes g_d odd. If \alpha,\beta\geq0, the first inequality in (4.12) bounds each term in (4.13) below by K/2.

If \alpha<0, set

u=-d\tan\alpha,\qquad v=d\tan\beta.

The inequality \alpha+\beta>0 gives \beta>-\alpha>0. Since the tangent is increasing on (-\pi/2,\pi/2), we have 0<u<v. Oddness and the second inequality in (4.12) give

\begin{aligned} g_d(d\tan\alpha)+g_d(d\tan\beta) &=g_d(v)-g_d(u)=\int_u^vG(d,s)\,\dd s\\ &\geq-\int_0^\infty\max\{0,-G(d,s)\}\,\dd s\geq K. \end{aligned}

The case \beta<0 is symmetric. Both endpoints cannot be negative because their sum is positive, so these cases are exhaustive.

Proposition 4.5 (From sector bounds to energy bounds). Let d_0>0, let I be finite or countable, let k_i\geq6 be integers with repetitions permitted, and let B,D_i\in C^1((0,\infty)) satisfy (4.3) and (4.4) with this lower distance d_0. For every sector (4.1) with d\geq d_0, use these same radial data in (4.5) and let J(S) be the functional (4.10). Suppose that K\leq0 and \lambda,\mu\in\R satisfy

\begin{aligned} J(S(d,\alpha,\beta)) &\geq K+\lambda A(S(d,\alpha,\beta))\\ &\qquad+\mu\theta(S(d,\alpha,\beta)), \end{aligned} \tag{4.14}

for every d\geq d_0, |\alpha|,|\beta|<\pi/2, and \alpha+\beta>0.

Compatible tori. Let \mathbb T=\R^2/\Gamma have area N, where N\geq1 is an integer. Suppose N distinct sites supply compatible periodic Voronoi data with lower edge distance d_0 and at most 6N face–edge sectors. Their mean-zero potential (4.7) satisfies

\mathcal W_{\mathbb T}(h)\geq N(6K+\lambda+2\pi\mu). \tag{4.15}

All square-torus configurations. Assume in addition d_0\leq d_*=1/(2\sqrt\pi). For every integer n\geq2 and every configuration of n distinct points v_1,\ldots,v_n on T_n=\R^2/(\sqrt n\,\Z^2), let h be the mean-zero solution of

-\Delta h=2\pi\left(\sum_{i=1}^n\delta_{v_i}-1\right).

Then its puncture-first energy (1.6), with embedded and pairwise disjoint punctures, satisfies

\mathcal W_n(h)\geq n(6K+\lambda+2\pi\mu). \tag{4.16}

More generally, if a periodic locally integrable field E on T_n satisfies, distributionally,

\operatorname{div}E=2\pi\left(\sum_{i=1}^n\delta_{v_i}-1\right), \qquad \operatorname{curl}E=0,

then E=-\nabla h+c for a constant c\in\R^2, and its energy with the same punctures and counterterm obeys

\mathcal E_{T_n}(E)=\mathcal W_n(h)+\frac n2|c|^2 \geq n(6K+\lambda+2\pi\mu).

The energy identity remains valid after applying the same fixed orthogonal rotation to both fields.

Proof. For compatible data, the sectors have total area N and total angle 2\pi N. Write M_0\leq6N for their number. Proposition 4.3 and (4.14) give

\begin{aligned} \mathcal W_{\mathbb T}(h) &\geq\sum_S J(S)\\ &\geq M_0K+\lambda N+2\pi\mu N\\ &\geq N(6K+\lambda+2\pi\mu). \end{aligned}

The last inequality uses M_0\leq6N and K\leq0; it includes K=0, when both terms involving K vanish.

Now assume d_0\leq d_* and fix n\geq2. Lemma 3.1 supplies a minimizing configuration of distinct points, with potential h_{\min}. Lemma 3.2 separates its full periodic lift by r_*=1/\sqrt\pi. Lemma 4.1 then gives at most 6n sectors, each with edge distance at least d_*\geq d_0. These are compatible data on T_n, so (4.15) applies to h_{\min}. Every other distinct configuration has energy at least \mathcal W_n(h_{\min}), proving (4.16) without a separation assumption on that configuration.

Equation (2.12) applies to the displayed divergence and curl conditions and gives the constant harmonic component and its exact energy penalty. A fixed orthogonal rotation preserves the squared norm and the puncture counterterm, giving the last assertion.

The next section chooses particular radial data and exact constants K<0,\lambda,\mu. For these data, the primitive identity (5.15) and the two scalar bounds yield

J(S)\geq K+\lambda A(S)+\mu\theta(S)

for every relevant sector. Proposition 5.4 applies the compatible-torus conclusion to this construction and identifies 6K+\lambda+2\pi\mu with the triangular energy. Section 8 uses the square-torus conclusion, whose minimizer argument has already removed the separation hypothesis.

5 Calibration on the triangular cell

We construct the radial functions used by the Voronoi test potential. The potential has the same gradient as the triangular Green function on a regular hexagon, while its energy on every other sector reduces to two scalar estimates. The continuation outside that hexagon is auxiliary; its explicit form makes those estimates accessible to interval arithmetic.

5.1 The local triangular Green function

Set

a=\sqrt{\frac{2}{\sqrt3}},\qquad p=\frac a2,\qquad R_0=\frac{2p}{\sqrt3},\qquad x_0=\frac{R_0}{2}. \tag{5.1}

Thus p and R_0 are the inradius and circumradius of the covolume-one triangular Voronoi hexagon, and x_0=p\tan(\pi/6). Identify the plane with \mathbb C, and write \partial_z=(\partial_x-i\partial_y)/2, with a nearest lattice point on the positive real axis. For m\ge1 put

k_m=6m,\qquad c_m=\frac1{k_m}\sum_{z\in\Lambda_\triangle\setminus\{0\}}z^{-k_m}. \tag{5.2}

These sums converge absolutely and are real by reflection symmetry. We also introduce an auxiliary index 0, with k_0=6. It is distinct from index 1: both exponents equal 6, but they will carry different radial functions.

Lemma 5.1. The mean-zero triangular Green function has the expansion

h_\triangle(z)=-\log|z|+C_\triangle+\frac{\pi|z|^2}{2} +\sum_{m\ge1}c_m\operatorname{Re}(z^{6m}), \qquad 0<|z|<a, \tag{5.3}

where C_\triangle is its regular part at the origin. The series and all of its derivatives converge locally away from |z|=a.

Proof. Away from the lattice, \Delta h_\triangle=2\pi, so 2\partial_z^2h_\triangle is a meromorphic elliptic function. Its double pole at each lattice point has principal part (z-\lambda)^{-2}. Subtract the absolutely locally convergent Weierstrass series

\wp(z)=\frac1{z^2}+\sum_{\lambda\ne0} \bigl((z-\lambda)^{-2}-\lambda^{-2}\bigr).

The difference is holomorphic and periodic, hence constant. If \omega=e^{\pi i/3}, invariance of h_\triangle under z\mapsto\omega z implies that its second complex derivative transforms by \omega^{-2}; the same is true of \wp. Their constant difference must therefore vanish. Expanding each summand for |z|<a gives

\wp(z)=z^{-2}+\sum_{j\ge1}(j+1)z^j \sum_{\lambda\ne0}\lambda^{-j-2}.

Rotation makes the inner sum zero unless j+2 is a multiple of 6. Twice complex differentiation of the right side of (5.3) gives this series, because k_m(k_m-1)c_m=(k_m-1)\sum\lambda^{-k_m}. The difference is a real harmonic affine function after subtracting \pi|z|^2/2; rotation removes its linear part and leaves C_\triangle. Normal convergence follows either from this power series or from the absolutely convergent lattice sums on every smaller disk.

5.2 Matching the regular hexagon

Write \gamma(r)=-\log r+\pi r^2/2 for r>0. We first choose the radial data on the regular hexagon, where the test potential must equal h_\triangle-C_\triangle. In a sector whose outward normal is the positive real axis, the edge has distance p and the endpoint angles are \pm\pi/6. At an edge point of radius t=p\sec\varphi,

p+i\sqrt{t^2-p^2}=te^{i|\varphi|}.

The boundary value of the mth Green-function mode is therefore c_mt^{k_m}\cos(k_m\varphi). Expressing it as a function of the radius gives the polynomial

V_m(r)=c_m\sum_{j=0}^{k_m/2}(-1)^j\binom{k_m}{2j} p^{k_m-2j}(r^2-p^2)^j, \qquad p\le r\le R_0. \tag{5.4}

On either vertex ray, the same mode equals (-1)^mc_mr^{k_m}, since k_m\pi/6=m\pi. This is the radial baseline we use for that mode inside the hexagon. The correction in (4.5) then recovers the angular dependence exactly:

(-1)^mc_mr^{k_m} +(r/t)^{k_m}\bigl(V_m(t)-(-1)^mc_mt^{k_m}\bigr) =c_mr^{k_m}\cos(k_m\varphi).

Thus the edge data b_m=V_m and the vertex-ray baseline determine the desired potential on each regular sector. Its remaining part \gamma is already radial and needs no correction there.

5.3 Continuation to arbitrary sectors

Other Voronoi sectors can have edge radii below p or above R_0. We now extend the radial data to those radii, keeping two derivatives and making the correction vanish beyond a fixed radius. The assembled potential is required to agree with h_\triangle-C_\triangle only inside the regular hexagon; the continuation is chosen for the scalar estimates, not as an extension of that Green function.

Define the clipped polynomial

S(y)=\begin{cases} 0,&y\le0,\\ 10y^3-15y^4+6y^5,&0<y<1,\\ 1,&y\ge1. \end{cases}

Let h_s=3/40 and c=3/50. For 0\le z\le h_s put

P(z)=z-\frac{6z^3}{h_s^2}+\frac{8z^4}{h_s^3}-\frac{3z^5}{h_s^4},\qquad Q(z)=\frac{z^2}{2}-\frac{3z^3}{2h_s} +\frac{3z^4}{2h_s^2}-\frac{z^5}{2h_s^3}.

For a function V with two left derivatives at R_0, its continuation is defined for r\ge R_0 by

(\mathcal HV)(r)= \begin{cases} V(R_0)+P(r-R_0)V'(R_0)+Q(r-R_0)V''(R_0),&r\le R_0+h_s,\\ V(R_0),&r>R_0+h_s. \end{cases} \tag{5.5}

Indeed (P,P',P'')(0)=(0,1,0) and (Q,Q',Q'')(0)=(0,0,1); all six values at h_s vanish. Thus this operation preserves two derivatives at R_0 and joins a constant with two derivatives at R_0+h_s.

Define b_0=\gamma up to R_0, continued by (5.5). For m\ge1, set b_m=V_m on [p,R_0] and use \mathcal HV_m above R_0. Below p put

b_m(r)=\begin{cases} 0,&0<r\le p-c,\\ S((r-p+c)/c)\bigl(T_{0m}+T_{1m}(r-p)+T_{2m}(r-p)^2\bigr),&p-c<r<p, \end{cases} \tag{5.6}

where

\begin{split} T_{0m}&=c_mp^{k_m},\\ T_{1m}&=-\frac{k_m(k_m-1)}pT_{0m},\\ T_{2m}&=\frac{k_m(k_m-1)}{p^2} \left(\frac{(k_m-2)(k_m-3)}6-\frac12\right)T_{0m}. \end{split}

Direct differentiation of (5.4) gives T_{0m}=V_m(p), T_{1m}=V_m'(p), and 2T_{2m}=V_m''(p). Consequently every b_i is C^2 away from the origin.

Now define

U_m(r)=(-1)^mc_mr^{k_m}\bigl(1-S((r-R_0)/(1/10))\bigr),\qquad \tau(r)=S\left(\frac{r-R_0-1/1000}{3/40}\right),

and set

\begin{split} u_0&=(1-\tau)\gamma+\tau b_0,\qquad u_m=(1-\tau)U_m+\tau b_m\quad(m\ge1),\\ B&=\sum_{i\ge0}u_i,\qquad D_i=b_i-u_i,\qquad l=R_0+\frac{19}{250}. \end{split} \tag{5.7}

Here the auxiliary mode 0 lets the radial part \gamma join its constant continuation by the same correction mechanism as the other modes. Its exponent k_0=6 makes this correction vanish at the pole without changing the singular normalization. The coefficient estimates proved below justify the sums and their first three derivatives on every open spline interval. In particular, B,D_i are C^2 and piecewise C^3 away from zero. Near zero, B=\gamma+\sum_{m\ge1}(-1)^mc_mr^{k_m}; normal convergence of (5.3) therefore gives

\begin{gathered} B(r)=-\log r+O(r^2),\qquad B'(r)=-1/r+O(r)\quad(r\downarrow0),\\ D_i(r)=0,\qquad B(r)=B(l)\quad(r\ge l). \end{gathered} \tag{5.8}

The fixed radial data also satisfy (4.4) for every d_0>0. Indeed, there are only finitely many retained modes, while for the omitted modes (6.4) and the vanishing of D_i beyond l bound the summand on [d_0,T_0] by (1+k_i+T_0)w_{k_i}. The explicit geometric terms in (6.3) make this series summable. This conclusion uses the analytic mode bounds, not the later finite-core estimates.

For a sector with edge distance d and endpoint angles -\alpha<\beta, write t(\varphi)=d\sec\varphi and use the test potential

H(r,\varphi)=B(r)+\sum_{i\ge0} \left(\frac r{t(\varphi)}\right)^{k_i}D_i(t(\varphi)), \qquad 0<r<t(\varphi),\quad -\alpha<\varphi<\beta. \tag{5.9}

At the edge its trace is \sum_i b_i(t); at a ray ending at a vertex of radius r_v its trace is B(r)+\sum_i(r/r_v)^{k_i}D_i(r_v). These expressions explain both trace matching conditions in the glued Voronoi construction.

5.4 The sector integral

The following formulas separate radial integration from sector geometry. For t>0 define

\begin{split} B_1(t)&=B'(t)+1/t,\qquad S_1(t)=\int_0^t B(r)r\,dr,\\ S_2(t)&=\int_0^t\bigl(-2B_1(r)+rB_1(r)^2\bigr)\,dr,\\ H_k(t)&=t^{-k}\int_0^tB_1(r)r^k\,dr,\qquad Q_i(t)=tD_i'(t)-k_iD_i(t). \end{split} \tag{5.10}

Here H_k is indexed by the exponent, so the two modes with exponent six use the same H_6. They remain separate in every sum involving D_i. Put

\begin{split} f_0(t)={}&-2\pi\left(S_1(t)+t^2\sum_i\frac{D_i(t)}{k_i+2}\right)\\ &-\frac12\Biggl(\log t+S_2(t) +\sum_i\bigl(-2D_i(t)+2k_iD_i(t)H_{k_i}(t)\bigr)\\ &\qquad+\sum_{i,j}\frac{k_ik_j}{k_i+k_j}D_i(t)D_j(t)\Biggr),\\ e(t)={}&\frac12\sum_{i,j}\frac{Q_i(t)Q_j(t)}{k_i+k_j}. \end{split} \tag{5.11}

All sums here and below include index 0. The angular coefficient is nonnegative, since

e(t)=\frac12\int_0^1 \left(\sum_iQ_i(t)v^{k_i}\right)^2\frac{dv}{v}\ge0. \tag{5.12}

Let J denote the sector contribution to the dual energy,

J=-2\pi\int_{\rm sector}H -\frac12\int_{\rm sector}^{\rm ren}|\nabla H|^2,

where the renormalized integral adds (\alpha+\beta)\log\eta before letting the radial exclusion \eta tend to zero. Then

J=\int_{-\alpha}^{\beta} \bigl(f_0(d\sec\varphi)-\tan^2\varphi\,e(d\sec\varphi)\bigr) \,d\varphi. \tag{5.13}

To verify this identity, differentiate (5.9):

H_r=-\frac1r+B_1(r)+\sum_i\frac{k_i}{r}(r/t)^{k_i}D_i(t),\qquad H_\varphi=\tan\varphi\sum_i(r/t)^{k_i}Q_i(t).

The source integral gives S_1+t^2\sum_iD_i/(k_i+2). The radial square contributes \log t+S_2, its cross terms contribute -2D_i+2k_iD_iH_{k_i}, and its quadratic terms have coefficient k_ik_j/(k_i+k_j). Integrating the angular square gives \tan^2\varphi\sum Q_iQ_j/(k_i+k_j). These are precisely (5.11). The estimates below permit termwise integration.

5.5 Subtracting area and angle

Given real constants \lambda,\mu, define

\begin{split} f(t)&=f_0(t)-\lambda t^2/2-\mu,\qquad t=\sqrt{d^2+s^2},\\ G(d,s)&=\frac d{t^2}f(t)-\frac{s^2}{dt^2}e(t),\qquad g_d(x)=\int_0^xG(d,s)\,ds\quad(d>0,\ x\in\mathbb R). \end{split} \tag{5.14}

The evenness of G in s makes g_d odd. If A is the sector area and \theta=\alpha+\beta, substitution s=d\tan\varphi in (5.13) gives

J-\lambda A-\mu\theta =g_d(d\tan\alpha)+g_d(d\tan\beta). \tag{5.15}

This identity holds for signed endpoint angles; only |\alpha|,|\beta|<\pi/2 and \alpha+\beta>0 are required.

We choose \lambda,\mu so that the adjusted primitive is stationary at the regular sector (d,x)=(p,x_0), and set K to twice its value there. The exact choices are

\begin{split} \lambda=\frac1{px_0}\biggl[&\frac p{x_0}\bigl(f_0(R_0)-f_0(p)\bigr) -\frac{x_0}{p}e(R_0)\\ &+p\int_0^{x_0}\frac{f_0(\sqrt{p^2+s^2})-f_0(p)}{s^2}\,ds +\frac1p\int_0^{x_0}e(\sqrt{p^2+s^2})\,ds\biggr],\\ \mu={}&f_0(R_0)-\frac13e(R_0)-\lambda R_0^2/2,\qquad K=2g_p(x_0). \end{split} \tag{5.16}

The first integrand extends continuously to s=0 with value f_0'(p)/(2p).

Lemma 5.2. For the constants (5.16), \nabla_{d,x}g_d(x)=0 at (p,x_0).

Proof. Let g_d^0 denote the primitive before subtracting area and angle. For fixed u=\pi/6, differentiation in the angle representation gives

\left.\frac d{dd}g_d^0(d\tan u)\right|_{d=p} =\int_0^{x_0}\frac{f_0'(t)-s^2e'(t)/p^2}{t}\,ds, \qquad t=\sqrt{p^2+s^2}.

Set V(s)=f_0(t)-f_0(p). Since V(s)=O(s^2), integration by parts has no boundary term at zero and yields

\int_0^{x_0}\frac{f_0'(t)}t\,ds =\frac{f_0(R_0)-f_0(p)}{x_0} +\int_0^{x_0}\frac{V(s)}{s^2}\,ds,

whereas

\int_0^{x_0}\frac{s^2e'(t)}{p^2t}\,ds =\frac{x_0e(R_0)}{p^2}-\frac1{p^2}\int_0^{x_0}e(t)\,ds.

The difference is the bracket in (5.16) divided by p, hence equals \lambda x_0. The subtracted area along x=d\tan u is \lambda d^2\tan u/2; its derivative at p is also \lambda x_0, and the subtracted angle is constant. Thus the derivative of g_d(d\tan u) vanishes there. Finally \partial_xg_p(x_0)=G(p,x_0)=0 by the definition of \mu, because x_0^2/p^2=1/3. The fixed-angle derivative is \partial_d+(x_0/p)\partial_x, so \partial_d vanishes as well.

Lemma 5.3. The calibrated constants satisfy

W(E_\triangle)=6K+\lambda+2\pi\mu. \tag{5.17}

Proof. Take \mathbb T=\R^2/\Lambda_\triangle and N=1. Its regular Voronoi hexagon supplies six compatible sectors with d=p and \alpha=\beta=\pi/6. The radial normalization and summability proved above supply the hypotheses of Proposition 4.3 with d_0=p, and the torus has area one. This application uses no square-torus minimizer or incidence theorem.

On each sector p\le t\le R_0, u_0(r)=\gamma(r) and u_m(r)=(-1)^mc_mr^{k_m} for r\le t. The edge trace and mode cancellation established above therefore give

H(r,\varphi)=\gamma(r)+\sum_{m\ge1}c_mr^{k_m}\cos(k_m\varphi) =h_\triangle-C_\triangle.

All six normals differ by multiples of \pi/3, which leaves these cosines unchanged. Hence \nabla H=\nabla h_\triangle and the nonnegative square in (4.11) is zero. Each sector has area 1/6 and angle \pi/3; its right side in (5.15) is 2g_p(x_0)=K. Summing the six contributions gives the cell energy 6K+\lambda+2\pi\mu. Lemma 2.3 identifies this cell energy with W(E_\triangle), proving (5.17).

5.6 The two scalar estimates needed by the geometry

The remaining analytic task is to establish

\begin{gathered} K<0,\qquad 2g_d(x)\ge K\quad(d\ge b,\ x\ge0),\qquad b=\frac{28209}{100000},\\ \int_0^\infty\max\{0,-G(d,s)\}\,ds\le-K\quad(d\ge b). \end{gathered} \tag{5.18}

The rational endpoint b=28209/100000 is below the geometric threshold d_*=1/(2\sqrt\pi). Thus the domain d\ge b covers all edge distances supplied by the separated-minimizer geometry; the elementary comparison is justified in Section 8.

The second estimate is essential when the perpendicular from a point to a Voronoi edge falls outside that edge. Its role is made precise in the following implication, which completes the geometric part of the argument once (5.18) has been certified.

Proposition 5.4. Assume (5.18) for the functions and constants just constructed. Let \mathbb T=\R^2/\Gamma be a flat torus of area N, where N\ge1 is an integer, and let v_1,\ldots,v_N be distinct sites. Suppose their full periodic lift gives compatible periodic Voronoi data with lower edge distance d_0=b and at most 6N face-edge sectors. Let h be the mean-zero potential (4.7), with energy \mathcal W_{\mathbb T}(h) defined by (4.8). Then

\mathcal W_{\mathbb T}(h)\ge NW(E_\triangle).

Proof. The radial normalization and compact summability established above supply the radial hypotheses of Proposition 4.5 with d_0=b. Evenness of G and (5.18) supply the hypotheses of Lemma 4.4 at this same lower distance. Combining its conclusion with (5.15) gives

J(S)\ge K+\lambda A(S)+\mu\theta(S)

for every sector with d\ge b, including the signed endpoint cases. The compatible-torus conclusion (4.15) now gives

\mathcal W_{\mathbb T}(h)\ge N(6K+\lambda+2\pi\mu) =NW(E_\triangle).

The equality is the exact triangular calibration (5.17), not a numerical estimate of the triangular energy.

6 Infinite-mode truncation and error propagation

This section supplies analytic estimates for the modes omitted after m=38. We use the radial functions b_m,U_m,u_m,B,D_m of the preceding construction, with

\begin{gathered} a=\sqrt{2/\sqrt3},\qquad p=a/2,\qquad R_0=a/\sqrt3,\\ b=\frac{28209}{100000},\qquad h_s=\frac{3}{40},\qquad c=\frac{3}{50},\qquad l=R_0+\frac{19}{250}. \end{gathered}

Thus k_0=6, k_m=6m for m\geq1, and

c_m=\frac1{k_m}\sum_{z\in\Lambda_\triangle\setminus\{0\}}z^{-k_m}.

Tildes will always mean that the modes m\geq39 have been omitted; the index-zero term is retained. Differences between a full quantity and its truncation are denoted by \Delta. Our goal is an absolute error below 10^{-11} for f_0,e and their first two derivatives on [b,l], conditional on the retained-mode bounds verified in Section 7.

6.1 Coefficient estimates

Write a lattice point as z=a(n+q/2+i\sqrt3 q/2), with (n,q)\in\Z^2. Then

|z/a|^2=n^2+nq+q^2\geq\frac34\max(|n|,|q|)^2.

There are 8v integer pairs with \max(|n|,|q|)=v. For every d=6m\geq6 and every positive integer D, the sum outside the square |n|,|q|\leq D, before multiplication by a^{-d}, is therefore at most

8(4/3)^{d/2}\sum_{v>D}v^{1-d} \leq 8(4/3)^{d/2}\frac{D^{2-d}}{d-2}. \tag{6.1}

The last inequality follows by comparison with the integral from D to infinity. The first shell has six points with squared norm 1 and two with squared norm 3. Moreover,

\sum_{v\geq2}v^{1-d} \leq 2^{1-d}+\int_2^\infty x^{1-d}\,\dd x =2^{1-d}\left(1+\frac2{d-2}\right) \leq3\,2^{1-d}.

It follows that, for d=k_m\geq12,

|c_m|\leq\frac{1}{d a^d} \left(6+2\,3^{-d/2}+24(4/3)^{d/2}2^{1-d}\right) \leq\frac7{d a^d}. \tag{6.2}

Indeed, the bracket equals 6+50/729<7 at d=12, and its two nonconstant terms decrease with d. The finite coefficient enclosures may use (6.1) with D=256 for m=1 and D=48 for 2\leq m\leq38, including the factor 1/(k_m a^{k_m}). Reflection symmetry makes each coefficient real.

6.2 Uniform derivative bounds for omitted modes

For k=6m\geq234, define the rational number

w_k=10^6\left( 30k^2(13/20)^k+3\cdot10^6 k^3 2^{-k} +5600k^5(3/5)^k+7\cdot10^{11}k^2(289/500)^k \right). \tag{6.3}

For 0\leq j\leq3 and 0<r\leq l, the construction satisfies

|u_m^{(j)}(r)|\leq w_k, \qquad |D_m^{(j)}(r)|\leq w_k. \tag{6.4}

At spline knots these inequalities mean both one-sided derivatives. Here are explicit checks of the constants.

The polynomial cutoff S(y)=10y^3-15y^4+6y^5 on [0,1], extended constantly outside that interval, obeys

|S|\leq1,\qquad |S'|\leq2,\qquad |S''|\leq6,\qquad |S'''|\leq60.

The identities p^4=1/12 and R_0^4=4/27 give the convenient rational bounds

.537<p<.538,\quad .620<R_0<.621,\quad .696<l<.697, \quad l/a<13/20,\quad R_0/a<289/500.

All terminating decimals in this section denote rational numbers.

For U_m(r)=(-1)^m c_mr^k(1-S((r-R_0)/.1)), Leibniz’ rule and (6.2) bound the third derivative by

7k^2(l/a)^k \left(l^{-3}+\frac{60}{kl^2} +\frac{1800}{k^2l}+\frac{60000}{k^3}\right).

Using l>.69 and k\geq234, the coefficient of k^2(13/20)^k is less than 25.445<30. The same calculation for orders 0,1,2 gives coefficients below 0.000001, 0.000197, and 0.070572, respectively. This proves the first term inside the parentheses in (6.3).

For p-c\leq r\leq p, write q_m(r)=T_{0m}+T_{1m}(r-p)+T_{2m}(r-p)^2, so that b_m(r)=S((r-p+c)/c)q_m(r). Since p/a=1/2 and p>1/2,

|T_{0m}|\leq\frac7k2^{-k},\qquad |T_{1m}|\leq14k2^{-k},\qquad |T_{2m}|\leq\frac{14}{3}k^3 2^{-k}.

The last inequality uses ((k-2)(k-3)/6)-1/2\leq k^2/6. Consequently

\begin{align*} |q_m|&\leq(7/k+.84k+.0168k^3)2^{-k},\\ |q_m'|&\leq(14k+.56k^3)2^{-k},\\ |q_m''|&\leq(28/3)k^3 2^{-k}.\end{align*}

In particular,

|b_m'''|\leq\frac{60}{c^3}|q_m| +\frac{18}{c^2}|q_m'|+\frac6c|q_m''| <8500k^3 2^{-k}<3\cdot10^6 k^3 2^{-k}.

The lower derivative orders satisfy the same final bound, and below p-c the function is zero.

On [p,p+.01], put w=r^2-p^2 and X=p+\sqrt w. The polynomial formula for V_m gives, for 0\leq\ell\leq3,

\left|\frac{\dd^\ell V_m}{\dd w^\ell}\right| \leq |c_m| k^{2\ell}X^{k-2\ell}.

For j\geq\ell, the coefficient comparison that proves this is

j(j-1)\cdots(j-\ell+1)\binom{k}{2j} \leq k^{2\ell}\binom{k-2\ell}{2j-2\ell}.

The bound p>.537 implies .02p+.0001<.04p^2, hence X\leq1.2p=(3/5)a on this interval. Also r<.55 and X>1/2. The chain rule gives

V_m'''(r)=8r^3\frac{\dd^3V_m}{\dd w^3} +12r\frac{\dd^2V_m}{\dd w^2}.

Thus its absolute value is at most

7\left(8(.55)^3 2^6+ \frac{12(.55)2^4}{234^2}\right)k^5(3/5)^k <597k^5(3/5)^k.

The lower derivatives satisfy smaller bounds. The common bound 5600k^5(3/5)^k therefore applies through order three.

On [p+.01,R_0], use z=p+i\sqrt{r^2-p^2}, so that V_m=\Re(c_mz^k) and |z|=r. Direct differentiation gives

|z'|\leq7,\qquad |z''|\leq300,\qquad |z'''|\leq60000.

For example, \sqrt{r^2-p^2}>.103, p<.54, and r<.63 suffice in the formulas |z'|=r/\sqrt{r^2-p^2}, |z''|=p^2/(r^2-p^2)^{3/2}, and |z'''|=3p^2r/(r^2-p^2)^{5/2}. Since 1/r<2, the third derivative of c_mz^k is bounded by

7\left(8\cdot343+\frac{12\cdot7\cdot300}{234} +\frac{2\cdot60000}{234^2}\right) k^2(289/500)^k <20000 k^2(289/500)^k.

All derivative orders through three are therefore bounded by 3\cdot10^6 k^2(289/500)^k on this interval.

For the extension \mathcal HV_m=V_m(R_0)+P(r-R_0)V_m'(R_0)+Q(r-R_0)V_m''(R_0), direct bounds on the coefficients of P,Q show, for 0\leq j\leq3,

|P^{(j)}|\leq2\cdot10^5,\qquad |Q^{(j)}|\leq4000.

Thus the common bound for the extension is at most

(1+200000+4000)\,3\cdot10^6 k^2(289/500)^k <7\cdot10^{11} k^2(289/500)^k.

It remains valid on the constant part beyond R_0+h_s.

Finally the cutoff \tau(r)=S((r-R_0-.001)/.075) satisfies

|\tau^{(j)}|\leq1,27,1067,142223 \qquad(j=0,1,2,3).

The maximal Leibniz factor through order three is 1+3\cdot27+3\cdot1067+142223=145506<10^6. Applying this to u_m=(1-\tau)U_m+\tau b_m and D_m=(1-\tau)(b_m-U_m) proves (6.4). The series and their indicated derivatives consequently converge absolutely and locally uniformly. For r<b, the omitted u_m derivatives additionally have their original O(r^{k-3}) behavior.

6.3 Norms and bounds for retained modes

For a function F with one-sided derivatives as needed, define

|F|_{j,t}=\sum_{q=0}^j\frac{|F^{(q)}(t)|}{q!}, \qquad \|F\|_{j,I}=\sup_{t\in I}|F|_{j,t}.

These norms are submultiplicative. For nonnegative weights \omega_i, a weighted mode norm means \sup_{t\in I}\sum_i\omega_i|F_i|_{j,t}: the sum is taken before the supremum.

The finite interval verification in Section 7 establishes the following bounds for the retained modes:

|\widetilde B_1|_{2,t}<6000, \qquad \sum_{i=0}^{38}(k_i+1)^3|\widetilde D_i|_{3,t}<2\cdot10^6, \qquad b\leq t\leq l. \tag{6.5}

The finite coefficient enclosure also supplies |c_1|<1. These assertions are not conclusions of the analytic estimates in this section. Conditional on them, the remaining estimates below are independent of the finite calculation.

On [0,b],

\widetilde B_1(t)=\pi t+ \sum_{m=1}^{38}(-1)^m k_mc_mt^{k_m-1}

has norm |\widetilde B_1|_{2,t}<10. For an explicit check, use t<b<2/7, a>1, \pi<22/7, and |c_1|<1 for the first mode. The modes k\geq12 contribute at most \sum_{k=12,18,\ldots}7k^2(2/7)^{k-3}<.014; the first term and its geometrically decreasing ratios prove this last rational inequality. Together with the linear term and the k=6 term this is less than 10.

6.4 Summing the omitted modes

Set

\mathfrak a=\sum_{k=234,240,\ldots}(k+1)^4w_k <2\cdot10^{-21},\qquad W_*=4\sum_{k=234,240,\ldots}w_k\leq4\mathfrak a. \tag{6.6}

Here is a rational verification of the numerical inequality. For each term (k+1)^4k^sr^k, with

(s,r)=(2,13/20),(3,1/2),(5,3/5),(2,289/500),

the ratio at the next allowed index is

\left(\frac{k+7}{k+1}\right)^4 \left(\frac{k+6}{k}\right)^s r^6.

It decreases with k, and at k=234 it is strictly below 1/10 for all four pairs. The first weighted summand obeys the exact rational comparison

\begin{split} 235^4\,10^6\bigl(&30\cdot234^2(13/20)^{234} +3\cdot10^6\cdot234^3 2^{-234}\\ &+5600\cdot234^5(3/5)^{234} +7\cdot10^{11}\cdot234^2(289/500)^{234}\bigr) <1.56\cdot10^{-21}. \end{split}

Multiplying by 10/9 gives a bound less than 2\cdot10^{-21}, as asserted in (6.6).

Since \Delta B_1=\sum_{m\geq39}u_m', the derivative estimates give

|\Delta B_1|_{2,t}\leq W_*,\qquad 0\leq t\leq l,

and, on [b,l],

\sum_{i\geq39}(k_i+1)^j|D_i|_{3,t}\leq4\mathfrak a, \qquad 0\leq j\leq4.

Indeed the divided-factorial sums use factors 5/2 and 8/3, respectively, both less than 4.

6.5 Propagation to the sector functions

Recall the quantities entering the sector formula:

\begin{align*} B_1(t)&=B'(t)+1/t,& S_1(t)&=\int_0^t B(r)r\,\dd r,\\ S_2(t)&=\int_0^t(-2B_1(r)+rB_1(r)^2)\,\dd r,& H_k(t)&=t^{-k}\int_0^t B_1(r)r^k\,\dd r,\\ Q_i(t)&=tD_i'(t)-k_iD_i(t).\end{align*}

Write N=2\cdot10^6 temporarily. Direct differentiation of \Delta S_1 gives

|\Delta S_1|_{2,t}\leq3W_*.

For example |\Delta B^{(j)}|\leq W_*/4 through order three, so the norm is at most [t^2/2+t+(1+t)/2]W_*/4 for t\leq l<1. For the other integral, use

\Delta(-2B_1+tB_1^2) =\bigl(-2+t(2\widetilde B_1+\Delta B_1)\bigr)\Delta B_1.

The second-order norm of its integral is at most twice the supremum of the first-order norm of the integrand, because l<1. Submultiplicativity and |t|_{1,t}<2 yield

|\Delta S_2|_{2,t} \leq(4+8\cdot6000+4W_*)W_*<60000W_*.

The identities and elementary bounds

H_k'=B_1-kH_k/t,\quad |H_k|\leq\frac{t\|B_1\|_{0,[0,t]}}{k+1},\quad |H_k'|\leq2\|B_1\|_{0,[0,t]},\quad |H_k''|\leq|B_1'|+\frac{2k}{t}\|B_1\|_{0,[0,t]}

imply, for b\leq t\leq l,

|H_k|_{2,t}\leq6(k+1)(6000+W_*),\qquad |\Delta H_k|_{2,t}\leq6(k+1)W_*. \tag{6.7}

Indeed l/(k+1)+5/2+k/b<6(k+1). The bound for \Delta H_k follows by the same linear argument applied to \Delta B_1.

The radial source and energy functions are

\begin{align*} f_0(t)={}&-2\pi\left(S_1(t)+t^2\sum_i\frac{D_i(t)}{k_i+2}\right)\\ &-\frac12\left(\log t+S_2(t) +\sum_i(-2D_i+2k_iD_iH_{k_i})(t) +\sum_{i,j}\frac{k_ik_j}{k_i+k_j}D_i(t)D_j(t)\right),\\ e(t)={}&\frac12\sum_{i,j}\frac{Q_i(t)Q_j(t)}{k_i+k_j}.\end{align*}

The preceding bounds give

\begin{align*} |f_0-\widetilde f_0|_{2,t} &\leq2\pi(3W_*+16\mathfrak a)\\ &\quad+\frac12\bigl(60000W_*+8\mathfrak a +12(2\cdot10^6)W_* +48(6000+W_*)\mathfrak a\\ &\hspace{44mm}+8(2\cdot10^6)\mathfrak a +16\mathfrak a^2\bigr) <6\cdot10^7\mathfrak a. \tag{6.8}\end{align*}

For completeness, |t^2|_{2,t}=(t+1)^2<4 gives the 16\mathfrak a source term. The sum of -2D_i contributes 8\mathfrak a. Split the mixed term as

\sum_i k_i(D_iH_{k_i}-\widetilde D_i\widetilde H_{k_i}) =\sum_{i\leq38}k_i\widetilde D_i\Delta H_{k_i} +\sum_{i\geq39}k_iD_iH_{k_i}.

The finite and omitted weighted norms give 12NW_* and 48(6000+W_*)\mathfrak a after including its factor 2. Bounding k_ik_j/(k_i+k_j) by k_ik_j, the quadratic difference is at most 8N\mathfrak a+16\mathfrak a^2. These are precisely the terms in (6.8). Finally W_*\leq4\mathfrak a, \pi<22/7, and \mathfrak a<2\cdot10^{-21} make its total coefficient less than 56,264,181<6\cdot10^7.

Since k_i\geq6 and t<1, direct differentiation of Q_i shows

|Q_i|_{2,t}\leq2(k_i+1)|D_i|_{3,t}.

For example, its coefficients on |D_i|,|D_i'|,|D_i''|,|D_i'''| are bounded respectively by k_i, t+k_i-1, t+(k_i-2)/2, and t/2. The finite and omitted sums of these norms are bounded by 2N and 8\mathfrak a. Dropping the denominator k_i+k_j\geq1 in the energy difference therefore gives

|e-\widetilde e|_{2,t} \leq16(2\cdot10^6)\mathfrak a+32\mathfrak a^2. \tag{6.9}

The norm contains half the absolute second derivative. Accounting for this factor, (6.8) and (6.9) imply absolute truncation errors less than 10^{-11} for every member of

f_0,\quad e,\quad f_0',\quad e',\quad f_0'',\quad e'' \qquad (b\leq t\leq l). \tag{6.10}

In fact the respective second derivative bounds are below 2.4\cdot10^{-13} and 1.3\cdot10^{-13}.

6.6 The constant region

For r\geq l, all D_i vanish and B is constant. The omitted constant satisfies

|\Delta B(l)|\leq \sum_{k=234,240,\ldots}\frac7k(R_0/a)^k \leq\frac{(7/234)(289/500)^{234}}{1-(289/500)^6} <6.075\cdot10^{-58}<10^{-11}.

Since B_1(t)=1/t there, the derivatives of \log t and S_2(t) cancel. The full infinite-mode functions consequently obey the exact formula

e(t)=0,\qquad f_0(t)=f_0(l)-\pi B(l)(t^2-l^2),\qquad t\geq l. \tag{6.11}

Thus outside [b,l] one propagates the enclosures of f_0(l) and B(l) through this exact formula; no uniform absolute error for arbitrarily large t is asserted.

7 The finite scalar verification

The geometric argument requires the two inequalities (5.18) for the exact functions G and g_d. We now specify a finite calculation that implies them. Its inputs are the radial data (5.7), the formulas (5.11), and the constants defined by the integrals (5.16). Its outputs are interval bounds for these constants, two strict bounds on a compact rectangle, and a positive Hessian bound near the exact stationary point. The estimates of Section 6 connect the finite radial calculation to the infinite series.

Every terminating decimal in this section denotes an exact rational number. An interval enclosure always contains the exact mathematical quantity in question. In particular, the constants \lambda,\mu,K are not replaced by rounded numerical choices. Their enclosures are used in all subsequent operations, while Lemma 5.2 supplies stationarity for their exact values.

7.1 Outward arithmetic and derivative intervals

The calculation follows the interval inclusion principle: every operation encloses its exact result, and analytic remainders are added explicitly. Revol and Rouillier [15] discuss this principle and the dependence of enclosure width on expressions and subdivision. We specify the integer operations here, so the proof’s arithmetic assumptions and rounding rules are explicit.

Put q=2^{144}. A scalar interval is represented by integers u\le v, meaning [u/q,v/q]. Rational inputs are rounded down at the lower endpoint and up at the upper endpoint. Addition and negation are exact at this denominator. Multiplication takes the least and greatest of the four endpoint products, then divides by q with outward rounding. If 0<u\le v, inversion gives

\left[\frac{\lfloor q^2/v\rfloor}{q}, \frac{\lceil q^2/u\rceil}{q}\right];

negative intervals are treated by negation, and division by an interval containing zero is forbidden. Integer powers use repeated multiplication. For a positive interval, integer square roots give the enclosure

\left[\frac{\lfloor\sqrt{uq}\rfloor}{q}, \frac{\lfloor\sqrt{vq}\rfloor+1}{q}\right].

The extra unit in the upper endpoint is harmless when the upper square root is an integer.

For logarithms, first extract an integer power of two and reduce the argument to [1/4,1]. The arguments used below are positive table intervals or enclosures of fixed positive constants; their widths allow this reduction. With z=(v-1)/(v+1), evaluate

\log v=2\sum_{j=0}^{199}\frac{z^{2j+1}}{2j+1}+\mathcal R, \qquad |\mathcal R| \le\frac{2(3/5)^{401}}{401(1-(3/5)^2)}<q^{-1}. \tag{7.1}

The same series at z=1/3 encloses \log2, used to restore the extracted power. All summation errors are already enclosed by outward arithmetic; the displayed remainder is added separately. Similarly, use

\pi=16\arctan(1/5)-4\arctan(1/239),\qquad \arctan(1/v)=\sum_{j=0}^{149} \frac{(-1)^jv^{-2j-1}}{2j+1}+\mathcal R_v. \tag{7.2}

The alternating-series bound gives |\mathcal R_v|\le v^{-301}/301<q^{-1} for both values of v. Adding [-2q^{-1},2q^{-1}] to each arctangent enclosure before the linear combination is sufficient. These procedures also enclose p,R_0,x_0,l using their exact defining formulas.

To bound derivatives we use interval jets

(F_0,F_1,F_2,F_3),\qquad F_j\supseteq F^{(j)}(t)/j!.

Addition, multiplication, inversion, logarithms, and square roots are performed as formal power series through degree three. For example, the product coefficient is \sum_{r=0}^jF_rG_{j-r}, and the inverse coefficients follow recursively from the product being one. A variable on a radial interval T is represented by (T,1,0,0); the resulting coefficients enclose its derivatives at every point of T on the chosen spline piece. At a single point, the leading interval encloses that point and the same derivative entries are used. After differentiation only the coefficients supported by the available derivative orders are used. The calculation below never requires a fourth derivative of a spline: third derivatives of B,D_i suffice for the second derivatives of f_0,e and for the radial quadrature errors.

For a differential equation Y'=F(t,Y) with an enclosed value at the evaluation point, its jet coefficients are reconstructed in increasing order by

Y_{j+1}=\frac{[F(t,Y)]_j}{j+1},\qquad 0\le j\le2. \tag{7.3}

Thus the enclosed value and the known differential equation supply the derivatives without numerical differentiation.

Spline polynomials are evaluated by interval Horner arithmetic. One may first translate a polynomial P(t)=\sum_{\ell=0}^Na_\ell t^\ell to the midpoint m of its leading interval:

P(m+h)=\sum_{j=0}^N \left(\sum_{\ell=j}^N\binom{\ell}{j}a_\ell m^{\ell-j}\right)h^j. \tag{7.4}

This is an exact polynomial identity, also for jets. It reduces interval widths without changing the spline or introducing an approximation; direct Horner evaluation remains a valid enclosure.

7.2 Coefficients and the radial table

Retain the auxiliary mode 0 and modes 1\le m\le38. The two modes with exponent six remain separate in sums involving D_i. Enclose each c_m by summing over |n|,|r|\le D, where D=256 for m=1 and D=48 otherwise, and then adding the symmetric error in (6.1), multiplied by a^{-k_m}/k_m. The summands can be evaluated using only integers before that last factor: if k=k_m, A=2n+r, and N=n^2+nr+r^2, then

\operatorname{Re}(n+r/2+i\sqrt3r/2)^{-k} =\frac{\displaystyle\sum_{j=0}^{k/2}(-1)^j \binom{k}{2j}A^{k-2j}(3r^2)^j}{2^kN^k}. \tag{7.5}

The pair (0,0) is omitted. The resulting enclosure also tests |c_1|<1.

The radial breakpoints are

b,\quad p-.06,\quad p,\quad R_0,\quad R_0+.001, \quad R_0+.075,\quad l=R_0+.076. \tag{7.6}

Each intervening interval is subdivided by affine interpolation between its exact endpoints. For the first interval use n=\lfloor8000(u-v)\rfloor+1 subintervals, and for all later intervals use n=\lfloor24000(u-v)\rfloor+1, where v,u are its endpoints. In execution an outward upper bound on the product is used to choose n, which can only add subdivisions. All true node positions are enclosed by the corresponding interval arithmetic. The length of every actual subinterval is bounded above in the calculation; these upper bounds are used in all error estimates.

For the fixed table, write [u_i/q,v_i/q] for the valid outward enclosure of its ith node, 0\le i\le m. The interval constructor enforces u_i\le v_i, and the node arithmetic preserves this invariant. After appending the last node and before propagating any integral state, the program requires

v_i<u_{i+1}\qquad(0\le i<m); \tag{7.7}

it throws an exception if a comparison fails. Thus, on a completed table construction, u_i\le v_i<u_{i+1}\le v_{i+1}. Both endpoint arrays are strictly increasing, and the stored step interval is

H_i=[(u_{i+1}-v_i)/q,(v_{i+1}-u_i)/q]

with positive lower endpoint. This also justifies every division by H_i below. These facts concern the initialized table and its unchanged aligned node, point, and cell arrays in the fixed calculation.

On 0<t\le p-.06, the truncated functions have the monomial form

\widetilde B(t)=-\log t+\pi t^2/2 +\sum_{m=1}^{38}a_mt^{k_m},\qquad \widetilde B_1(t)=\pi t+\sum_{m=1}^{38}k_ma_mt^{k_m-1}, \qquad a_m=(-1)^mc_m.

For compact formulas introduce the finite list

(e_0,v_0)=(2,\pi),\qquad (e_m,v_m)=(k_m,k_ma_m)\quad(1\le m\le38).

This list indexes monomials of \widetilde B_1, rather than the sector modes; its exponent e_0=2 is unrelated to k_0=6. The starting integrals, including their derivatives, are obtained from the exact identities

\begin{split} \widetilde S_1(t)&=\frac{t^2}{2}\left(\frac12-\log t\right) +\frac\pi8t^4+ \sum_{m=1}^{38}\frac{a_mt^{k_m+2}}{k_m+2},\\ \widetilde S_2(t)&=-2\sum_{i=0}^{38}\frac{v_it^{e_i}}{e_i} +\sum_{i,j=0}^{38}\frac{v_iv_jt^{e_i+e_j}}{e_i+e_j},\\ \widetilde H_k(t)&=\sum_{i=0}^{38}\frac{v_it^{e_i}}{e_i+k}. \end{split} \tag{7.8}

In particular, the table starts propagation at the exact node p-.06 with these values; preceding nodes and cells use (7.8) directly.

There is a useful exact simplification for the sector functions on this first interval. Since b_m(t)=0, D_m(t)=-a_mt^{k_m} and D_0(t)=0, substitution in (5.9) cancels every nonconstant mode and gives H(r,\varphi)=\gamma(r) for r\le t. Equivalently, every Q_i vanishes. Direct radial integration gives

f_0(t)=(\pi t^2-\tfrac12)\log t-\frac{3\pi^2t^4}{8}, \qquad e(t)=0,\qquad 0<t\le p-.06. \tag{7.9}

Indeed,

\int_0^t\gamma(r)r\,\mathrm dr =-\frac{t^2}{2}\log t+\frac{t^2}{4}+\frac{\pi t^4}{8}, \qquad \int_0^t{}^{\rm ren}\gamma'(r)^2r\,\mathrm dr =\log t-\pi t^2+\frac{\pi^2t^4}{4}.

Combining these with the source and energy factors in the sector formula proves (7.9). The identity holds for the full infinite series as well as for every finite truncation. It may therefore replace the mode sums when evaluating f_0,e and their first two derivatives on the first interval, producing tighter enclosures. The full finite-mode values (7.8) at p-.06 are still required to start the continuation of S_1,S_2,H_k.

For a subsequent radial step [v,u], propagate the integrals by

\begin{split} \widetilde S_1(u)&=\widetilde S_1(v)+ \int_v^u r\widetilde B(r)\,\mathrm dr,\\ \widetilde S_2(u)&=\widetilde S_2(v)+ \int_v^u\bigl(-2\widetilde B_1(r) +r\widetilde B_1(r)^2\bigr)\,\mathrm dr,\\ \widetilde H_k(u)&=(v/u)^k\widetilde H_k(v) +\int_v^u(r/u)^k\widetilde B_1(r)\,\mathrm dr. \end{split} \tag{7.10}

For each integrand Y, the midpoint rule has the rigorous enclosure

\int_v^uY(r)\,\mathrm dr \in (u-v)Y((v+u)/2) +\left[-\frac{(u-v)^3}{24}\sup_{[v,u]}|Y''|, \frac{(u-v)^3}{24}\sup_{[v,u]}|Y''|\right]. \tag{7.11}

Midpoint values use point jets; second-derivative bounds use a jet whose leading interval contains [v,u]. The formula applies to weak second derivatives bounded almost everywhere as well.

For values inside a step, use the integral equations rather than the midpoint approximation. If T=[v,u] and h=u-v, then

\begin{split} \widetilde S_j(T)&\subseteq \widetilde S_j(v) +[0,h]\,\operatorname{range}_T Y_j, \qquad j=1,2,\\ \widetilde H_k(T)&\subseteq (v/T)^k\widetilde H_k(v) +[-h\|\widetilde B_1\|_{0,T}, h\|\widetilde B_1\|_{0,T}], \end{split} \tag{7.12}

where Y_1=r\widetilde B and Y_2=-2\widetilde B_1+r\widetilde B_1^2. For the last inclusion, (r/t)^k\le1 whenever v\le r\le t\le u. Recover the positive jet orders from

\widetilde S_1'=t\widetilde B,\qquad \widetilde S_2'=-2\widetilde B_1+t\widetilde B_1^2,\qquad \widetilde H_k'=\widetilde B_1-k\widetilde H_k/t. \tag{7.13}

Substitution into (5.11) produces both node enclosures and cell enclosures of the ordered six-tuple

(\widetilde f_0,\widetilde f_0',\widetilde f_0'', \widetilde e,\widetilde e',\widetilde e''). \tag{7.14}

No numerical differentiation of table values is used.

Separately, subdivide each interval in (7.6) into steps of length at most .00022. Direct interval jets for \widetilde B_1 and \widetilde D_i test the two finite-core inequalities (6.5). Together with |c_1|<1, these are the finite premises of the truncation analysis; their verification does not use any infinite-mode error bound. Only after these tests pass is (6.10) invoked.

The spline data are C^2 and have bounded one-sided third derivatives. Accordingly f_0,e are C^1 with locally bounded weak second derivatives on (b,\infty). A radial cell uses its own spline formula at its endpoints; either one-sided second derivative is valid for its interior. When a query meets a knot, the hull includes both adjacent cells. Thus no jump of a second derivative is mistaken for global classical differentiability.

7.3 Queries for the infinite-mode functions

Let \epsilon=[-10^{-11},10^{-11}], and let T be a valid outward enclosure of the queried true radii. In the fixed production calls every such radius is at least b, although T may extend below b. For derivatives, take the componentwise hull of (7.14) over every radial cell meeting T and add \epsilon to each component. By (6.10), this encloses the full infinite-mode tuple (f_0,f_0',f_0'',e,e',e'') at every queried true radius in T\cap[b,l]. The exact continuation below covers queried true radii at least l. Here is the cell-selection argument for the implementation. In integer endpoint units write the valid query as [a,b'], let j be the first index with v_j\ge a, and let k be the first index with u_k>b', using m+1 if either index is absent. The closed envelope of cell i is [u_i,v_{i+1}]. It meets [a,b'] exactly when v_{i+1}\ge a and u_i\le b'. By the ordering proved above, these conditions are equivalent to i\ge j-1 and i<k. Therefore the binary searches on the upper and lower endpoint arrays select exactly

\mathrm{im}=\max(0,j-1)\le i<\min(m,k)=\mathrm{ix}.

The non-strict intersection inequalities include both cells at a shared endpoint. Every true cell meeting the query lies in its envelope and is therefore selected; any extra cells only widen the hull. This is a statement about the fixed initialized table, not a general-purpose lookup interface.

For a query requiring values alone, improve the enclosure by linear interpolation of the endpoint values. On a radial cell [v,u] put

X=[0,1]\cap\frac{T-v}{u-v},\qquad L_Y(T)=Y(v)+X\bigl(Y(u)-Y(v)\bigr), \quad Y=\widetilde f_0,\widetilde e.

An empty intersection is discarded. The interpolation error is

|Y(t)-L_Y(t)|\le\frac{(u-v)^2}{8} \sup_{[v,u]}|Y''|. \tag{7.15}

The cell enclosure supplies the derivative bound. Add this symmetric error and \epsilon, then take the hull over all relevant cells. Shared coefficient uncertainties need not be independent: interval operations enclose all their possible values and hence also their correlated exact values. In particular, the positive stored interval H_i contains the true step u-v, so outward evaluation of the quotient defining X contains the normalized coordinate of every true queried point in that cell. Intersecting with [0,1] cannot discard such a point.

Queries that meet [l,\infty) also include the exact continuation (6.11). Enclose its two constants by the last node value plus \epsilon and by

B(l)\in-\log R_0+\pi R_0^2/2+ \sum_{m=1}^{38}V_m(R_0)+\epsilon. \tag{7.16}

Thus the continuation contributes the tuple

\bigl(f_0(l)-\pi B(l)(T^2-l^2),\, -2\pi B(l)T,\,-2\pi B(l),\,0,0,0\bigr). \tag{7.17}

Using the entire query interval in this expression is conservative even if it extends below l, since the relevant exterior subset is contained in it. This rule propagates the constant uncertainties through the exact formula and asserts no radius-independent error on the unbounded tail.

7.4 Enclosing the calibrated constants

We evaluate the exact integrals defining \lambda in (5.16). Put s_0=.01 and t(s)=\sqrt{p^2+s^2}. Taylor’s formula at p removes the apparent division by zero in the first integral. Specifically,

\begin{split} \int_0^{s_0}p\frac{f_0(t(s))-f_0(p)}{s^2}\,\mathrm ds \in{}& f_0'(p)\left(\frac{s_0}{2} -\frac{s_0^3}{24p^2} +\left[0,\frac{s_0^5}{80p^4}\right]\right)\\ &+\frac{s_0^3}{6} \left[\frac{p}{(\sqrt{p^2+s_0^2}+p)^2},\frac1{4p}\right] \operatorname{range}_{[p,t(s_0)]} f_0''. \end{split} \tag{7.18}

Indeed, t-p=s^2/(t+p), while

\frac{p}{t+p}=\frac12-\frac{s^2}{8p^2} +\left[0,\frac{s^4}{16p^4}\right].

The quadratic Taylor remainder of f_0 supplies the second line of (7.18). The derivative range comes from the radial cells with the infinite-mode error added.

The implementation obtains this range by a direct cell scan over [p,t(s_0)], and obtains the derivative bounds below by a second direct scan over [p,R_0]. Both use the same closed-cell selection rule, with outward endpoint bounds, but neither adds the exterior formula. This is sufficient here: p^4=1/12 gives p>1/2>b, x_0=R_0/2>s_0, and

t(x_0)=\sqrt{p^2+(R_0/2)^2}=R_0<l.

Hence both true scan domains are contained in the finite table [b,l]. A nonempty scan alone would not justify a query extending beyond that table.

On [s_0,x_0] integrate p(f_0(t(s))-f_0(p))/s^2 by a midpoint sum with 45000 equal steps. Integrate e(t(s))/p on [0,x_0] by a separate midpoint sum with 45000 equal steps. Obtain integer upper bounds

C\ge\sup_{[p,R_0]}|f_0'|,\quad C'\ge\sup_{[p,R_0]}|f_0''|,\quad E\ge\sup_{[p,R_0]}|e'|,\quad E'\ge\sup_{[p,R_0]}|e''|

from the cell enclosures plus \epsilon. The two integrands have second derivatives bounded respectively by

\frac{C'}p+\frac{8C}{s_0^2},\qquad \frac{E'}p+\frac E{p^2}. \tag{7.19}

For the first bound, set V=f_0(t(s))-f_0(p); then

|V|\le Cs^2/(2p),\qquad V''=f_0''(t)(s/t)^2+f_0'(t)p^2/t^3,

and differentiate pV/s^2 twice. The resulting terms are p(V''/s^2-4V'/s^3+6V/s^4), bounded by the first expression in (7.19). The second follows by twice differentiating e(t(s))/p. For an interval of length L and equal step length h, add the symmetric error Lh^2\sup|Y''|/24 to each complete midpoint sum. Together with (7.18), the endpoint terms and the factors in (5.16), this encloses \lambda. The same formula then encloses \mu.

To enclose K=2\int_0^{x_0}G(p,s)\,\mathrm ds, choose an integer n and equal steps of length h=x_0/n\le.0001, and use their midpoint sum. Independently enclose G_{ss}(p,s) on a partition with step length at most .0002. If h is the midpoint step length and L_K bounds this second derivative, the enclosure is

K\in2\left(\sum_jhG(p,s_j) +[-x_0h^2L_K/24,x_0h^2L_K/24]\right). \tag{7.20}

The factor two multiplies both the sum and its error.

The first sign tests are

\begin{gathered} -6.731<\lambda<-6.729,\qquad K<0,\\ f_0(l)-\lambda l^2/2-\mu>0,\qquad -\pi B(l)-\lambda/2>0. \end{gathered} \tag{7.21}

Each strict inequality is accepted only when the corresponding interval endpoint proves it. The bound on \lambda also serves as a check on the normalization. The last two signs and (6.11) give

f(t)=f(l)+\bigl(-\pi B(l)-\lambda/2\bigr)(t^2-l^2)>0, \qquad G(d,s)>0\quad\hbox{if }t=\sqrt{d^2+s^2}\ge l. \tag{7.22}

Here e(t)=0 and d/t^2>0.

7.5 The compact rectangle and its derivative bounds

Because l<.697 and \sqrt{b^2+.65^2}>l, the signs (7.22) reduce the remaining work to

\mathcal D=[b,.697]\times[0,.65]. \tag{7.23}

For d\ge.697, G(d,s)>0 for every s\ge0 and g_d(x)\ge0. For d\ge b and x\ge.65, the primitive is increasing in x. The negative part of G vanishes for s\ge.65.

We obtain derivatives of G by differentiating its defining formula, using the full radial query enclosures. The following identities specify all needed factors. Put

t=\sqrt{d^2+s^2},\quad A=d/t^2,\quad Z=-s^2/(dt^2)=A-1/d,\quad r_d=d/t,\quad r_s=s/t,

and write f'=f_0'-\lambda t, f''=f_0''-\lambda. Then

\begin{aligned} A_d&=(1-2d^2/t^2)/t^2,&Z_d&=A_d+1/d^2,\\ A_s&=-2ds/t^4,&Z_s&=A_s,\\ A_{dd}&=2d(d^2-3s^2)/t^6,&Z_{dd}&=A_{dd}-2/d^3,\\ A_{ss}&=-2d/t^4+8ds^2/t^6,&Z_{ss}&=A_{ss}. \end{aligned} \tag{7.24}

For v=d or v=s let r_v have the meaning above. The derivative formulas are

\begin{split} G_v={}&A_vf+Af'r_v+Z_ve+Ze'r_v,\\ G_{vv}={}&A_{vv}f+2A_vf'r_v +A\bigl(f''r_v^2+f'(1-r_v^2)/t\bigr)\\ &+Z_{vv}e+2Z_ve'r_v +Z\bigl(e''r_v^2+e'(1-r_v^2)/t\bigr). \end{split} \tag{7.25}

These formulas hold on each smooth piece and almost everywhere across the radial knots. No mixed second derivative of G is needed.

Partition both sides of (7.23) into intervals of length at most .0008. Interval substitution in (7.25) on every closed rectangle supplies global upper bounds

L_1\ge\|G_d\|_{\infty,\mathcal D},\quad L_2\ge\|G_s\|_{\infty,\mathcal D},\quad L_3\ge\|G_{dd}\|_{\infty,\mathcal D},\quad L_4\ge\|G_{ss}\|_{\infty,\mathcal D}. \tag{7.26}

The value-only interpolation is not used to obtain these derivative bounds.

7.6 The primitive away from its stationary point

Let

\mathcal D_0=[.52528,.54930]\times[.29420,.32621]. \tag{7.27}

Its interior contains (p,x_0). To verify the primitive bound on the complement, partition the d interval at the two vertical sides of \mathcal D_0, and partition the s interval at its two horizontal sides. Subdivide these pieces into steps with maximal lengths

D_h\le.00019,\qquad S_h\le.00018.

Every cell therefore lies either in \mathcal D_0 or outside its interior. For each d node, form successive midpoint sums from 0 to every x node, using the actual step lengths:

Q(d,x)=\sum_{[s_j,s_{j+1}]\subseteq[0,x]} (s_{j+1}-s_j) G\left(d,\frac{s_j+s_{j+1}}2\right).

The sum at x=0 is zero and is tested as well. The value queries in Section 7.3 may be used here. At every node outside the interior of \mathcal D_0, enclose 2Q(d,x)-K and let m_* be a lower bound for all these enclosures.

The quadrature error at grid nodes is bounded by E_0, and the additional interpolation error between nodes by E_I, where

E_0=\frac{2(.65)S_h^2L_4}{24},\qquad E_I=\frac{2\bigl(D_h^2(.65)L_3+S_h^2L_2\bigr)}8, \tag{7.28}

Indeed, the bilinear interpolation estimate follows from

\partial_d^2(2g_d(x)-K)=2\int_0^xG_{dd}(d,s)\,\mathrm ds, \qquad \partial_x^2(2g_d(x)-K)=2G_s(d,x).

Apply the one-dimensional interpolation error in each variable successively; the resulting bounds add and require no mixed derivative. Thus the finite assertion

m_*-E_0-E_I>0 \tag{7.29}

proves 2g_d(x)>K throughout \mathcal D\setminus\operatorname{int}\mathcal D_0. All the derivative estimates are weak derivative estimates, so the same conclusion holds when a quadrature segment or rectangle crosses a radial knot.

7.7 The negative part on the whole rectangle

At every d node, including those between the vertical sides of \mathcal D_0, use the same s partition to enclose

N(d)=\sum_j(s_{j+1}-s_j) \max\left\{0,-G\left(d,\frac{s_j+s_{j+1}}2\right)\right\}.

Let N_* be an upper bound for all these sums. The function y\mapsto\max\{0,-y\} is 1-Lipschitz. On a subinterval of length h, its midpoint error is therefore at most L_2h^2/4: integrate L_2|s-s_{\rm mid}|. Summing the errors gives at most .65S_hL_2/4. Every d lies within D_h/2 of a node; changing d to that node changes the integral by at most .65D_hL_1/2. Consequently the assertion

N_*+K+.65\left(\frac{S_hL_2}{4}+\frac{D_hL_1}{2}\right)<0 \tag{7.30}

proves

\int_0^{.65}\max\{0,-G(d,s)\}\,\mathrm ds<-K \qquad(b\le d\le.697).

Together with (7.22), this gives the entire negative-part inequality in (5.18).

7.8 Convexity in the stationary rectangle

It remains to prove the primitive inequality on \mathcal D_0. Partition its d interval into steps of length at most .00004. Partition [0,.32621] into steps of length at most .00008, including .29420 as a node. The accumulation in s must begin at zero even though the Hessian is tested only above .29420.

For a d interval D and an s interval S_j, use the full derivative queries to enclose

F_1(D,S_j)\supseteq G_{dd}(D,S_j),\quad F_2(D,S_j)\supseteq G_d(D,S_j),\quad F_3(D,S_j)\supseteq G_s(D,S_j).

For a cell D\times S_j meeting \mathcal D_0, enclosures of the three Hessian entries of (d,x)\mapsto g_d(x) are

\begin{split} A_j&=\sum_{i<j}|S_i|F_1(D,S_i) +[0,|S_j|]F_1(D,S_j),\\ B_j&=F_2(D,S_j),\qquad C_j=F_3(D,S_j). \end{split} \tag{7.31}

The first line is direct interval integration, not midpoint quadrature: it bounds both the completed subintervals and the partial final subinterval. Test, on every such cell, that

\inf A_j>0,\qquad \inf C_j>0,\qquad \inf(A_jC_j-B_j^2)>0. \tag{7.32}

Interval multiplication encloses the determinant even when its factors are correlated. These inequalities imply positive definiteness, and in particular positive semidefiniteness, of the Hessian almost everywhere on \mathcal D_0.

The function (d,x)\mapsto g_d(x) belongs to W^{2,\infty} on a neighbourhood of this rectangle. To justify the passage from Hessian bounds to convexity, mollify on each smaller interior rectangle: the mollified Hessian is positive semidefinite, so the mollified functions are convex. Local uniform convergence proves convexity in the interior, and continuity includes the boundary. By Lemma 5.2, (p,x_0) is an interior stationary point. Hence

2g_d(x)\ge2g_p(x_0)=K\qquad((d,x)\in\mathcal D_0). \tag{7.33}

This step uses the exact stationary point and does not infer convexity or stationarity from sampled function values.

7.9 Finite assertions and the scalar conclusion

For clarity, the finite procedure has the following fixed parameters and obligations.

QuantityParameter or required assertion
ArithmeticDenominator 2^{144}, jet order 3
Retained modesi=0,1,\ldots,38
Coefficient squaresD=256 for m=1, D=48 otherwise
Core meshAt most .00022 on each spline interval
Core assertions|c_1|<1 and (6.5)
Radial tableDensities 8000 and 24000 as specified above
Radial node orderingStrict separation (7.7) at every adjacent pair
\lambda integrals45000 midpoint steps each; s_0=.01
K integralSteps at most .0001; derivative mesh .0002
Exterior signsAll assertions in (7.21)
Global derivative meshAt most .0008 in both coordinates
Outer and negative-part meshD_h\le.00019, S_h\le.00018
Outer and negative-part assertions(7.29), (7.30)
Hessian meshd steps .00004, s steps .00008 or smaller
Hessian assertions(7.32) on every cell

Proposition 7.1 (Meaning of the finite assertions). Apply the outward interval procedure specified in this section to the radial data (5.7), retaining modes 0 through 38, with the parameters in the table. If every listed assertion holds, its enclosures establish the finite-core premise (6.5), the exterior positivity (7.22), the primitive bound outside the interior of \mathcal D_0, the negative-part bound for every d\ge b, and the convexity bound (7.33), all for the exact infinite-mode functions.

Proof. The coefficient sum and its lattice tail enclose each retained coefficient. The direct core tests concern only finitely many modes, so they imply the premise needed for (6.10). Equations (7.8)–(7.13) and the midpoint bound prove the node and cell table enclosures by induction through every radial step. The node-separation guard supplies the positive steps and ordered search arrays used by the table and query arguments. The query rules then enclose the exact infinite-mode functions and their first two derivatives, including the constant-region continuation.

The origin expansion and midpoint errors prove the enclosures of \lambda,\mu,K. The signs (7.21) imply the positive tail. The derivative bounds, quadrature errors and bilinear interpolation prove the outer primitive assertion; the Lipschitz estimate proves the negative-part assertion. Finally, (7.31) encloses the complete Hessian, whose positivity and exact stationarity give (7.33). Every stage uses only enclosures established before that stage.

Finite bounds. The program certificate.cpp implements this procedure using core.hpp and grids.hpp. All three files and an execution wrapper are included in the verification directory. One completed guarded run is documented in verification/README.md, which binds the code and formula hashes, run metadata, saved integer pairs, and their interpretation below. The wrapper compiles and runs the computation; it does not read the TeX manuscript. The source-to-code and analytic correspondences are separate arguments. The interval denominator is 2^{144}. The table gives outward-rounded projections, while interval assertions use uncoarsened endpoints.

QuantityRecorded projection
\lambda[-6.7300312,-6.7300275]
\mu[.4138830,.4138838]
K[-.0034823,-.0034809]
B(l)[1.0464643,1.0464644]
f_0(l)[-1.2135966,-1.2135965]
f(l)[.0044755,.0044772]
-\pi B(l)-\lambda/2[.0774490,.0774509]
m_*-E_0-E_I\ge .0000120
Negative-part left side of (7.30)\le -.0004585
g_{dd} on \mathcal D_0\ge1.0529222
g_{xx} on \mathcal D_0\ge .0128335
\det\nabla^2g on \mathcal D_0\ge .0086252

Here the determinant is enclosed on each individual rectangle before the bounds are combined; it is not computed from separately combined entry ranges. The global derivative bounds, rounded outwards for display, are

L_1\le7.4636170,\qquad L_2\le2.5091315,\qquad L_3\le143.7890461,\qquad L_4\le315.1489689.

These derivative numbers are projections of the computed hulls, not separate executable threshold assertions. For the identified sources, under the documented runtime assumptions, the completed run verifies the listed finite assertions using uncoarsened interval endpoints. Proposition 7.1 explains why these assertions imply the required bounds for the exact infinite-mode functions: the interval formulas and range-coverage arguments identify the quantities enclosed, while the analytic truncation estimates supply the omitted modes. Neither the rounded table nor the execution record alone supplies those mathematical correspondences.

Theorem 7.2 (Scalar inequalities from the finite verification). The exact constants and functions of (5.16) and (5.14) satisfy

K<0,\qquad 2g_d(x)\ge K\quad(d\ge b,\ x\ge0),\qquad \int_0^\infty\max\{0,-G(d,s)\}\,\mathrm ds\le-K \quad(d\ge b).

Proof. The documented finite verification and the correspondences just established supply the hypotheses of Proposition 7.1. The first assertion is part of (7.21). The outer-grid assertion and (7.33) cover all of \mathcal D. For d\in[b,.697] the positive tail makes the primitive increasing after x=.65, so the primitive bound extends to every x\ge0. For d\ge.697, G(d,s)>0 for all s\ge0, whence g_d(x)\ge0>K/2. The negative-part estimate follows from (7.30) on the rectangle; its integrand vanishes outside the rectangle by (7.22). These are exactly (5.18).

8 The finite-torus and whole-plane bounds

We now apply the geometric comparison to the certified scalar bounds, then pass from square tori to the plane. The square-torus conclusion of Proposition 4.5 already incorporates the separation of minimizers and the passage to arbitrary configurations.

Proof of Theorem 1.2. The radial data of Section 5 satisfy (4.3)–(4.4) with lower distance d_0=b=28209/100000. Theorem 7.2 gives K<0 and both bounds in (5.18). By Lemma 4.4 at d_0=b and the primitive identity (5.15), these bounds give (4.14) for every sector with d\geq b, including the signed endpoint cases.

Since b<1/(2\sqrt\pi)=d_*, as follows from \pi<3.1416, the square-torus conclusion of Proposition 4.5 applies. For every n\geq2 and every configuration of n distinct points it gives, using the exact triangular calibration (5.17),

\mathcal W_n(h)\geq n(6K+\lambda+2\pi\mu)=nW(E_\triangle).

No separation hypothesis is imposed on this configuration. The same proposition gives the energy penalty n|c|^2/2 for a constant harmonic component and preserves the bound under a fixed orthogonal rotation.

Proof of Theorem 1.1. The periodic triangular field belongs to the admissible class and has finite energy by Lemmas 2.1 and 2.3. Thus C=W(E_\triangle) is a finite real number. Apply Proposition 2.4 to Theorem 1.2 with this C. It gives the lower bound for every field in the stated admissible class and for each fixed cutoff family (1.1). The triangular field attains the lower bound.

The comparison establishes the minimum of this logarithmic renormalized energy. It does not classify all configurations having that energy per unit area. In particular it supplies no uniqueness or defect-exclusion assertion.

8.1 The spherical logarithmic-energy constant

Proof of Corollary 1.3. Write \mathcal A_m^{\mathrm{BS}} and W_{\mathrm{ball}} for the admissible class and ball-cutoff energy of Bétermin and Sandier [1, Definitions 2.1–2.4]. Their fields satisfy \operatorname{div}E=2\pi(\nu_\Lambda-m) and \curl E=0, with the same charge-growth condition and local puncture functional as here. At m=1 the admissible class is our \mathcal A_1; the local integrability conventions agree by Lemma 2.1. The outer average, however, is over centered balls rather than squares.

The component rotation j\mapsto F=(j_2,-j_1) is a bijection from \mathcal C_1 to \mathcal A_{1/(2\pi)}^{\mathrm{BS}} and preserves the local energy. Thus (2.2) identifies M with \min_{\mathcal A_{1/(2\pi)}^{\mathrm{BS}}}W_{\mathrm{ball}}. The scaling formula [1, equation (2.4)] gives

\min_{\mathcal A_1^{\mathrm{BS}}}W_{\mathrm{ball}} =2\pi\left(M-\frac14\log(2\pi)\right). \tag{8.1}

Lemma 2.2 bounds every square-cutoff energy W(E) below by the right-hand side. Conversely, periodic averaging applied to the scaled square-periodic sequence in the proof of Proposition 2.4 shows that its square-cutoff energies converge to that value. Theorem 1.1 therefore identifies it with W(E_\triangle). This uses the common ball and square minimum in (2.2), not equality of those two energies for an arbitrary field. Lemma 2.3 does give equality for the periodic field E_\triangle, so this covolume-one triangular field attains the minimum in (8.1). Its value also agrees with the periodic lattice notation in Bétermin and Sandier: replacing their gradient \nabla H_\Lambda by the admissible field -\nabla H_\Lambda leaves the local squared-norm functional unchanged.

Theorem 1.5 of [1] gives the form of (1.7) with C in place of C_{\mathrm{BHS}}, where

C=\frac1\pi\min_{\mathcal A_1^{\mathrm{BS}}}W_{\mathrm{ball}} +\frac12\log\pi+\log2,

and states that C=C_{\mathrm{BHS}} exactly when the density-one triangular lattice attains this minimum. Its energy is precisely the ordered-pair sum on the unit sphere in \R^3 used here. In particular, the -n(n-1)\log2 term in its passage from the radius-1/2 sphere to the unit sphere contributes both -n^2\log2 and +n\log2; no further pair-counting or radius factor is needed. The equality clause now gives (1.8) and proves the corollary.

A Supplementary coefficient and tail estimates

The proof uses the coefficient enclosures and omitted-mode estimates in Sections 6 and 7. This appendix records an independent integer recurrence for the same finite coefficient sums and alternative exact bounds for the same omitted-mode series. These arguments are supplementary: they do not add a hypothesis to the scalar theorem or replace the analytic derivative bounds and finite retained-mode premises used there.

A.1 An independent recurrence for the lattice coefficients

Fix integers (n,q)\ne(0,0) and write

A=2n+q,\qquad N=n^2+nq+q^2,\qquad \zeta=A+i\sqrt3q,\qquad w=\frac{\zeta}{2}.

Thus w=n+q/2+i\sqrt3q/2, N=|w|^2>0, and |\zeta|^2=4N. A point of the covolume-one triangular lattice is aw, where a=\sqrt{2/\sqrt3}. For m\geq0, put

r_m(n,q)=\operatorname{Re}(\zeta^{6m}).

The two numbers u=\zeta^6 and v=\overline{\zeta}^{6} have

u+v=2r_1,\qquad uv=(4N)^6,

and hence satisfy X^2-2r_1X+(4N)^6=0. Multiplying this equation by u^{m-1} and v^{m-1}, respectively, and adding gives the integer recurrence

\begin{split} r_0&=1,\\ r_1&=A^6-45A^4q^2+135A^2q^4-27q^6,\\ r_{m+1}&=2r_1r_m-(4N)^6r_{m-1}\qquad(m\geq1). \end{split} \tag{A.1}

Here all the quantities on the right are integers. This proves the recurrence for every individual lattice point, without a numerical approximation to a complex power.

The binomial theorem identifies its numerator exactly. Since only even powers of i\sqrt3q have nonzero real part,

r_m(n,q)=\sum_{j=0}^{3m}(-1)^j\binom{6m}{2j} A^{6m-2j}(3q^2)^j. \tag{A.2}

This is the numerator in (7.5), after writing q for its second integer coordinate. Indeed, w^{-6m}=\overline{w}^{6m}/N^{6m}, and therefore

\operatorname{Re}(w^{-6m}) =\frac{r_m(n,q)}{2^{6m}N^{6m}} =\frac{r_m(n,q)}{(64N^6)^m}. \tag{A.3}

Thus the recurrence and the binomial expression agree for every point and every mode, not only for a selected finite list of comparisons.

Grouping by the norm. For a positive integer D, let

\mathcal Q_D=\{(n,q)\in\Z^2:\ |n|,|q|\leq D,\ (n,q)\ne(0,0)\}, \qquad R_{m,N}(D)=\sum_{\substack{(n,q)\in\mathcal Q_D\\n^2+nq+q^2=N}} r_m(n,q).

After forming the numerator for each point, one may combine the equal denominators in (A.3):

\sum_{(n,q)\in\mathcal Q_D}\operatorname{Re}(w^{-6m}) =\sum_{N\geq1}\frac{R_{m,N}(D)}{(64N^6)^m}. \tag{A.4}

Only finitely many positive norms occur. It is important that the recurrence precede this grouping. For fixed D, summing (A.1) over a norm shell gives

R_{m+1,N}(D) =2\sum_{\substack{(n,q)\in\mathcal Q_D\\n^2+nq+q^2=N}} r_1(n,q)r_m(n,q)-(4N)^6R_{m-1,N}(D).

In general the first sum cannot be replaced by one value of r_1 times R_{m,N}(D). For example, (7,0) and (5,3) both have N=49, but their respective values of r_1 are 7\,529\,536 and -4\,912\,064. One may apply the recurrence either pointwise or within groups having the same pair (N,r_1), and only then combine all terms of a common norm.

For the finite coefficient enclosures, take D=256 when m=1 and D=48 when 2\leq m\leq38. The omitted dimensionless sum has absolute value at most

E_{m,D}=8(4/3)^{3m}\frac{D^{2-6m}}{6m-2}

by (6.1). The coefficient c_m is consequently enclosed by adding [-E_{m,D},E_{m,D}] to the finite sum in (A.4) and then multiplying by the positive factor a^{-6m}/(6m). The square and its omitted tail are unchanged by grouping.

Complex pairs and interval containment. The finite calculation may instead keep both real components. Write

\zeta^6=r_1+i\sqrt3\,s_1,\qquad s_1=6A^5q-60A^3q^3+54Aq^5.

The multiplication rule

(x+i\sqrt3y)(x'+i\sqrt3y') =(xx'-3yy')+i\sqrt3(xy'+yx')

shows that, starting from (x_0,y_0)=(1,0),

(x_{m+1},y_{m+1}) =(x_mr_1-3y_ms_1,\ x_ms_1+y_mr_1)

represents \zeta^{6(m+1)} exactly. In particular x_m=r_m and its real component obeys (A.1). This is the complex-pair recursion used in the finite calculation, again applied per point before norm grouping. The half square n>0, or n=0 and q>0, contains one point of each pair (n,q),(-n,-q). Because 6m is even, the two real numerators agree, which justifies doubling each half-square contribution.

For completeness, grouping also explains an interval containment relation. At fixed denominator Q=2^{144}, let

\mathcal I_Q(x)= \left[\frac{\lfloor Qx\rfloor}{Q}, \frac{\lceil Qx\rceil}{Q}\right] \qquad(x\in\mathbb Q).

For any finite rational list x_1,\ldots,x_h, the elementary inequalities

\left\lfloor\sum_jQx_j\right\rfloor\geq\sum_j\lfloor Qx_j\rfloor, \qquad \left\lceil\sum_jQx_j\right\rceil\leq\sum_j\lceil Qx_j\rceil

give

\mathcal I_Q\left(\sum_jx_j\right) \subseteq\sum_j\mathcal I_Q(x_j). \tag{A.5}

Apply this to the exact rationals in each norm shell. Converting the shell sum once and then summing shells is contained in the enclosure obtained by converting every point separately. Adding the same outward tail interval and multiplying by the same positive scaling enclosure preserve containment, because interval addition, multiplication, and outward rounding are monotone under inclusion. This statement assumes the same primitive rounding rule, tail enclosure, and scaling enclosure on both sides; exact algebra alone does not assert endpoint identity or containment between different choices of those enclosures.

A.2 Alternative exact bounds for the omitted modes

For the allowed indices k=234,240,\ldots, split the weighted summand (k+1)^4w_k of (6.3) into four positive rationals:

\begin{align*} t_1(k)&=10^6\,30(k+1)^4k^2(13/20)^k,\\ t_2(k)&=10^6(3\cdot10^6)(k+1)^4k^3(1/2)^k,\\ t_3(k)&=10^6\,5600(k+1)^4k^5(3/5)^k,\\ t_4(k)&=10^6(7\cdot10^{11})(k+1)^4k^2(289/500)^k.\end{align*}

Then

\mathfrak a=\sum_{j=0}^{\infty}\sum_{i=1}^4t_i(234+6j).

This is the same \mathfrak a as in (6.6), distinct from the lattice scale a. If

(p_i,\beta_i)=(2,13/20),(3,1/2),(5,3/5),(2,289/500),

in the order i=1,2,3,4, the exact consecutive ratios are

\rho_i(k)=\frac{t_i(k+6)}{t_i(k)} =\left(\frac{k+7}{k+1}\right)^4 \left(\frac{k+6}{k}\right)^{p_i}\beta_i^6. \tag{A.6}

Both rational factors decrease for k>0, so each \rho_i(k) decreases. The four initial ratios, with no rounding, are

\begin{array}{c|c} i&\rho_i(234)\\ \hline 1&(241/235)^4(40/39)^2(13/20)^6\\ 2&(241/235)^4(40/39)^3(1/2)^6\\ 3&(241/235)^4(40/39)^5(3/5)^6\\ 4&(241/235)^4(40/39)^2(289/500)^6. \end{array}

Here is an exact simultaneous check that all four are less than 1/10. The integer comparisons

\begin{align*} 9\cdot241^4=30\,360\,623\,049 &<30\,498\,006\,250=10\cdot235^4,\\ 7\cdot40^5=716\,800\,000 &<721\,793\,592=8\cdot39^5,\\ 800\cdot13^6=3\,861\,447\,200 &<4\,032\,000\,000=63\cdot20^6\end{align*}

give, since p_i\leq5 and 0<\beta_i\leq13/20,

\rho_i(234) \leq(241/235)^4(40/39)^5(13/20)^6 <\frac{10}{9}\frac87(13/20)^6<\frac1{10} \quad(1\leq i\leq4). \tag{A.7}

Three geometric bounds. Set T_0=\sum_{i=1}^4t_i(234). One convenient entirely integer form of its exact comparison is obtained by putting

\begin{align*} C_{234}={}&30\cdot234^2\cdot325^{234} +3\cdot10^6\cdot234^3\cdot250^{234}\\ &+5600\cdot234^5\cdot300^{234} +7\cdot10^{11}\cdot234^2\cdot289^{234}.\end{align*}

The common denominator 500^{234} gives

T_0=\frac{10^6\,235^4 C_{234}}{500^{234}},\qquad 10^{29}235^4 C_{234}<156\cdot500^{234}.

The displayed integer inequality is exactly T_0<156/10^{23}. In particular,

\frac{10}{9}T_0<\frac{1560}{9\cdot10^{23}} <\frac2{10^{21}}, \tag{A.8}

where the last comparison reduces to 1560<1800.

Let \rho_{\max}=\max_{1\leq i\leq4}\rho_i(234), and define three exact rational upper bounds

A_{\rm coarse}=\frac{10}{9}T_0,\qquad A_{\rm common}=\frac{T_0}{1-\rho_{\max}},\qquad A_{\rm component}=\sum_{i=1}^4 \frac{t_i(234)}{1-\rho_i(234)}.

Decreasing ratios imply t_i(234+6j)\leq t_i(234)\rho_i(234)^j. Summing these geometric majorants and using (A.7) proves

\mathfrak a\leq A_{\rm component} \leq A_{\rm common}<A_{\rm coarse}<\frac2{10^{21}}. \tag{A.9}

The second inequality holds because 1-\rho_i(234)\geq1-\rho_{\max}>0. The common-ratio estimate keeps only the largest initial ratio, whereas the componentwise estimate retains each one; both refine the coarse factor 10/9.

An exact partial sum and a positive remainder bound. There are exactly 62 allowed indices from 234 through 600, because 600=234+6\cdot61. Define the finite rational sum

P_{600}=\sum_{i=1}^4\sum_{j=0}^{61}t_i(234+6j) \tag{A.10}

and the positive rational number

R_{606}=\sum_{i=1}^4\frac{t_i(606)}{1-\rho_i(606)},\qquad \rho_i(606)=\left(\frac{613}{607}\right)^4 \left(\frac{102}{101}\right)^{p_i}\beta_i^6. \tag{A.11}

Every numerator is positive and 0<\rho_i(606)<\rho_i(234)<1/10, so R_{606}>0. Starting the geometric estimate at the next mode 606, rather than at the last included mode 600, gives

P_{600}<\mathfrak a\leq P_{600}+R_{606}. \tag{A.12}

The first inequality is strict because all subsequent summands are positive. The number R_{606} is an upper bound for the remainder, not an assertion that the remainder equals it.

This refinement is no larger than the componentwise bound. For the i-th component put r=\rho_i(234). Then t_i(606)\leq t_i(234)r^{62} and \rho_i(606)\leq r, while each term of its partial sum is at most t_i(234)r^j. Consequently

\sum_{j=0}^{61}t_i(234+6j) +\frac{t_i(606)}{1-\rho_i(606)} \leq t_i(234)\left(\sum_{j=0}^{61}r^j+ \frac{r^{62}}{1-r}\right) =\frac{t_i(234)}{1-r}.

Summing over i places P_{600}+R_{606} below A_{\rm component} in (A.9). These finite bounds are exact rationals; a rounded display that makes P_{600} and P_{600}+R_{606} look equal does not change (A.12).

Rational propagation to the radial errors. The refined bounds can be substituted directly into the propagation estimates of Section 6.5. They do not replace its analytic mode bounds or the finite premises (6.5): the retained second-order B_1 norm is still bounded by 6000, and the weighted third-order D_i norm by 2\cdot10^6. Recall also that

W_*=4\sum_{k=234,240,\ldots}w_k \leq4\sum_{k=234,240,\ldots}(k+1)^4w_k=4\mathfrak a, \tag{A.13}

so replacing W_* by 4\mathfrak a is an upper bound, not an identity. Collecting the integral and mode-norm contributions in (6.8) and using \pi<22/7 gives the rational expression, for A,W\geq0,

\begin{align*} \mathcal F(A,W)={}&2\frac{22}{7}(3W+16A)\\ &+\frac12\bigl(60000W+8A+12(2\cdot10^6)W +48(6000+W)A\\ &\hspace{30mm}+8(2\cdot10^6)A+16A^2\bigr). \tag{A.14}\end{align*}

The terms are respectively the source integral, the S_2 error, the linear D_i error, the retained and omitted mixed D_iH_{k_i} errors, and the quadratic D_iD_j error. The bound \pi<22/7 and (6.8) give |f_0-\widetilde f_0|_{2,t}\leq\mathcal F(\mathfrak a,W_*). Every coefficient of \mathcal F is nonnegative. Thus any one of the rational upper bounds A above, for which \mathfrak a\leq A, satisfies

|f_0-\widetilde f_0|_{2,t} \leq\mathcal F(\mathfrak a,W_*)\leq\mathcal F(A,4A).

Direct collection of the rational terms gives the exact identity

\mathcal F(A,4A)=A\bigl(56\,264\,180+104A\bigr). \tag{A.15}

For example, the source term contributes 176A; the remaining linear terms contribute 56\,264\,004A, and the quadratic terms contribute 104A^2.

Put A_0=2/10^{21}. Each rational upper bound for \mathfrak a above is less than A_0, and the coefficient in (A.15) increases with A. The exact comparison

56\,264\,180+\frac{208}{10^{21}} <56\,264\,181<6\cdot10^7

therefore supplies the claimed coefficient bound. More explicitly,

\mathcal F(A_0,4A_0) =\frac{112\,528\,360}{10^{21}}+\frac{416}{10^{42}} <\frac{12}{10^{14}}.

The order-two norm is |F|_{2,t}=|F(t)|+|F'(t)|+|F''(t)|/2. Hence the second derivative, unlike the value and first derivative, requires the factor 2:

|f_0''-\widetilde f_0''| \leq2|f_0-\widetilde f_0|_{2,t} <\frac{24}{10^{14}}=2.4\cdot10^{-13}.

For the angular function, (6.9) similarly yields the entirely rational comparison

|e''-\widetilde e''| \leq2\bigl(16(2\cdot10^6)A_0+32A_0^2\bigr) =\frac{128\,000\,000}{10^{21}}+\frac{256}{10^{42}} <\frac{13}{10^{14}}=1.3\cdot10^{-13}.

The value and first derivative are bounded by their norms without this factor. Thus these rational alternatives preserve the error threshold 10^{-11} for all six quantities in (6.10) on [b,l]. For t\geq l, the exact continuation (6.11), rather than a uniform absolute error at unbounded radius, remains the applicable statement.

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