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Equality cases in the sharp one-dimensional matrix Lieb–Thirring inequality

OpenAI, 5 October 2026

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Abstract

We classify all equality cases in the sharp one-dimensional Lieb–Thirring inequality for every finite matrix size and 1/2<\gamma<3/2. For measurable Hermitian positive semidefinite potentials W with \int_\R\tr(W^{\gamma+1/2})<\infty, equality holds precisely for direct sums, in one constant unitary basis, of scalar one-bound-state solitons and zero channels. The nonzero solitons may have independent scales and centers.

1 Introduction

Lieb–Thirring inequalities compare the binding energy of a Schrödinger operator with an integral of its potential. Equality asks how the potential must arrange that binding. In one dimension, a scalar one-bound-state optimizer has a hyperbolic-secant profile. For a matrix potential, several such profiles can occupy orthogonal internal channels. The issue is whether equality also permits channels that rotate with position, or several bound states that interact within the same channel. We prove that throughout 1/2<\gamma<3/2 every equality case consists of independent scalar profiles in one fixed basis.

Let m\ge1 be finite, let 1/2<\gamma<3/2, and set p=\gamma+1/2. For a measurable Hermitian positive semidefinite function W:\R\to\C^{m\times m} satisfying

\int_\R\tr(W(x)^p)\,dx<\infty, \tag{1.1}

let H_W=-d^2/dx^2-W be the operator associated with

h_W[\psi]=\int_\R\|\psi'\|^2 -\int_\R\langle\psi,W\psi\rangle, \qquad \psi\in H^1(\R;\C^m). \tag{1.2}

Lemma 2.1 proves that the form is closed and bounded below and that the negative spectrum is discrete, with possible accumulation only at zero. We write

\Tr(H_W)_-^\gamma=\sum_{\lambda_j(H_W)<0}|\lambda_j(H_W)|^\gamma,

counting multiplicities. The finite-dimensional trace \tr is unnormalized; matrix powers are defined by spectral functional calculus.

Theorem 1.1 (Equality classification). For every W satisfying (1.1),

\Tr(H_W)_-^\gamma\le C_\gamma\int_\R\tr(W^p), \qquad C_\gamma=\left(\frac{\gamma-1/2}{\gamma+1/2}\right)^{\gamma-1/2} \frac{\Gamma(\gamma+1)}{\sqrt\pi\,\Gamma(\gamma+3/2)}. \tag{1.3}

Put r=(\gamma-1/2)^{-1}. Equality holds if and only if there are k\in\{0,\ldots,m\}, a constant unitary matrix U, positive numbers a_1,\ldots,a_k, and real numbers x_1,\ldots,x_k such that almost everywhere

W(x)=U\diag\bigl(w_1(x),\ldots,w_k(x),0,\ldots,0\bigr)U^*, \quad w_j(x)=(r+1)a_j^2\sech^2\!\bigl(ra_j(x-x_j)\bigr). \tag{1.4}

The case k=0 means W=0. Each nonzero channel has exactly one negative eigenvalue, -a_j^2, and therefore every extremal potential has at most m negative eigenvalues, counted with multiplicity.

The inequality in (1.3) is the sharp matrix inequality of [11, Theorem 1.1]. Our contribution is its equality classification. We retain the analytic constructions in the proof, so that the inequality and its equality conditions are established here under the same measurable potential hypothesis. The scales and centers in (1.4) are independent; repeated scales and identical profiles are allowed.

1.1 History and related results

Lieb and Thirring introduced spectral moment inequalities in their work on the kinetic energy of fermions and stability of matter [8, 9]. Their sharp constants distinguish the regimes in which binding is best concentrated in a single state or distributed among many states. Keller’s optimization of the lowest Schrödinger eigenvalue [6] supplies the one-state problem underlying the scalar profiles in (1.4); their explicit form appears in [9, Section 4(B), Equations (4.19)–(4.20)]. The present question concerns equality in the sum of all negative eigenvalue moments, with a matrix potential that need not commute with itself at different points.

The sharp scalar endpoint \gamma=1/2 was proved by Hundertmark, Lieb and Thomas [5]; Hundertmark, Laptev and Weidl [4, Theorem 3.1] extended it to operator-valued potentials. The semiclassical constant is sharp for \gamma\ge3/2; the lifting of moments of Aizenman and Lieb [1] and the operator-valued inequalities of Laptev and Weidl [7] are central to this development. Benguria and Loss [2] gave a commutation proof of the matrix result at \gamma=3/2. More recently, Read and Schulz [12] proved the sharp scalar inequality at \gamma=1, with constant 4/(3\sqrt3\pi), and its operator-valued extension. The matrix companion [11] proves the sharp one-state constant for the whole open interval considered here.

The endpoint \gamma=3/2 has a different equality structure. In the scalar finite-rank problem, Frank, Gontier and Lewin [3, Theorem 5] identify the optimizers as KdV multisolitons. In particular, several bound states can occur in a single scalar channel at that endpoint. The conclusion of Theorem 1.1, one bound state per nonzero channel, uses the strict inequality r>1 and is asserted only for the open interval.

1.2 Quantitative defects and fixed channels

The proof begins with the finite-interval matrix action method of [11]. For orthonormal real trial functions approximating finitely many negative eigenfunctions, place the functions in the rows of U(x) and choose a lower triangular matrix C. The rows of A=CU remain in the successive trial spans. If K is the diagonal matrix of positive square roots of the trial binding energies, the action involves A', K^2AA^T, and a power of the density AA^T. A symmetric matrix path B(x) connects K to -K and gives a lower bound for that action.

For equality, the lower bound must retain more information. Besides the square \|A'-BA\|_{\HS}^2, we retain a term controlling

[B,K^2]\quad\hbox{and}\quad K^2-B^2-(AA^T)^r.

Its coefficient depends on the largest binding energy and the exponent, but not on the number of trial functions. This uniformity is the first essential point: an extremal potential is not known in advance to have finitely many negative eigenvalues. The integrated trace identity of the matrix companion supplies the two nonnegative squares from which this estimate follows.

The second point is compactness with a fixed number of columns. As the trial list grows, A has more rows but still only m columns. Its density therefore has rank at most m. The retained defect bounds the tail rows by the small binding energies in that tail. This yields strong pointwise convergence even for an infinite eigenvalue list and gives exact algebraic relations in the limit. Those relations separate the rows with different energies. A differential inequality then makes their row spaces independent of position; their mutual orthogonality leaves at most m nonzero directions. On each resulting finite block, a matrix Riccati equation has a fixed diagonalizing basis and determines the profiles in (1.4).

Section 2 gives the spectral and convexity preliminaries. Section 3 proves the quantitative action estimate, and Section 4 recovers the sharp spectral bound. Section 5 passes to exact relations for an equality case. Section 6 proves that the channels are fixed, solves the Riccati equation, and treats complex potentials and the converse. Appendices A and B prove the trace identity, regularized field construction, and connecting-path theorem used by the action estimate.

1.3 Notation

Throughout the proof,

\sigma=\gamma-\tfrac12\in(0,1),\qquad p=1+\sigma,\qquad r=\sigma^{-1},\qquad q=r+1, \tag{1.5}

and

D_\sigma=\frac{\sigma^\sigma}{(1+\sigma)^{1+\sigma}},\qquad b_\sigma=\int_{-1}^1(1-s^2)^\sigma\,ds,\qquad C_\gamma=\frac{D_\sigma}{b_\sigma}. \tag{1.6}

The last identity follows from the beta integral. We use the operator norm \|\cdot\|_{\op} and the Hilbert–Schmidt norm \|A\|_{\HS}^2=\tr(A^*A). The symbol T denotes transpose of a real matrix, and \Sym_n is the space of real symmetric n\times n matrices with inner product \tr(BH). The commutator is [B,H]=BH-HB. The identity matrix, or identity operator, has the size determined by its context.

2 Spectral and convexity preliminaries

Two elementary facts let us work with measurable potentials and identify the equality condition in the potential estimate. The first is the form argument used in the matrix inequality [11, Lemma 7.1]; we give its proof to fix the precise regularity available below.

Lemma 2.1. Let p>1 and let W:\R\to\C^{m\times m} be measurable, Hermitian and positive semidefinite, with \int_\R\tr(W^p)<\infty. The form h_W on H^1(\R;\C^m) is closed and bounded below. Multiplication by W^{1/2} is compact from H^1 to L^2. The negative spectrum of H_W consists of isolated eigenvalues of finite multiplicity, with possible accumulation only at zero. Its eigenfunctions belong to H^1 and satisfy -\psi''-W\psi=\lambda\psi distributionally.

Proof. Set w=\|W\|_{\op}. Then w^p\le\tr(W^p), so w\in L^p. The one-dimensional Sobolev estimate, applied to the norm of a vector function, gives \|\psi\|_\infty^2\le2\|\psi\|_2\|\psi'\|_2. Hölder’s inequality, interpolation and Young’s inequality imply

\int_\R\langle\psi,W\psi\rangle \le 2^{1/p}\|w\|_p\|\psi'\|_2^{1/p}\|\psi\|_2^{2-1/p} \le \varepsilon\|\psi'\|_2^2+C_\varepsilon\|\psi\|_2^2. \tag{2.1}

A sufficiently shifted form norm is therefore equivalent to the H^1 norm. This proves closedness and semiboundedness, and polarization gives continuity of the potential form on H^1.

Write T\psi=W^{1/2}\psi. The truncated multiplier T_{R,L}=\mathbf1_{\{|x|\le R,\,w\le L\}}T is compact by the compact embedding of H^1([-R,R]) into L^2([-R,R]). Moreover,

\|(T-T_{R,L})\psi\|_2^2 \le C\|w\mathbf1_{\{|x|>R\}\cup\{w>L\}}\|_p\|\psi\|_{H^1}^2.

The coefficient tends to zero, so T is compact. For each a>0, an infinite-dimensional spectral subspace in (-\infty,-a] would contain an L^2-orthonormal sequence bounded in H^1 by (2.1). A subsequence converges weakly to zero in H^1, hence its images under T converge strongly to zero. This contradicts -a\ge h_W[\psi]\ge-\|T\psi\|_2^2 for unit vectors in that subspace. Thus every such subspace is finite-dimensional. Finally, the weak form equation tested against smooth compactly supported functions is the stated distributional equation; its potential term is locally integrable because W\in L^p_{\mathrm{loc}} and \psi is locally bounded.

Lemma 2.2 (Trace Young inequality and its equality condition). For positive semidefinite matrices W,Z of the same finite size, set

Y(W,Z)=D_\sigma\tr(W^p)-\tr(WZ)+\tr(Z^q). \tag{2.2}

Then Y(W,Z)\ge0, with equality if and only if W=qZ^r. Also,

Y(W,Z)\ge\tfrac12\tr(Z^q) -(2^{p-1}-1)D_\sigma\tr(W^p). \tag{2.3}

Proof. Scalar maximization over z\ge0 gives yz-z^q\le D_\sigma y^p for y\ge0, with equality precisely when y=qz^r. In an orthonormal eigenbasis (v_j) of Z, let z_j be its eigenvalues and put y_j=\langle v_j,Wv_j\rangle. Strict convexity of t^p on [0,\infty) gives

\tr(WZ)-\tr(Z^q) \le D_\sigma\sum_j y_j^p \le D_\sigma\sum_j\langle v_j,W^pv_j\rangle.

Equality in the second inequality holds exactly when each v_j belongs to an eigenspace of W. Equality in the first then requires Wv_j=qz_j^rv_j for every j. This proves both directions of the equality assertion, including zero eigenvalues. Applying the same inequality to 2W,Z gives \tr(WZ)\le\tfrac12\tr(Z^q)+2^{p-1}D_\sigma\tr(W^p), which is (2.3).

3 An action estimate that retains the equality defects

The finite-interval argument for the sharp inequality can also measure failure of its equality relations. We retain the first-order square and a quantitative part of the matrix trace deficit. The coefficient of this second defect will be independent of the number of rows. This uniformity allows us to exhaust an eigenvalue list before knowing that it is finite.

The construction adapts the field, connecting paths, and action identity of [11, Sections 3–6]. Their analytic foundations are proved in Appendices A and B; the additional estimate below extracts operator-norm rigidity from the trace deficit.

Fix positive integers n,d, a bounded interval \Omega=(x_-,x_+), and K=\operatorname{diag}(\ell_1,\ldots,\ell_n) with 0<\ell_i\leq\kappa. For A\in H^1_0(\Omega;\R^{n\times d}), set \rho=AA^{\mathsf T} and define

\mathcal E_K(A)=\int_\Omega \bigl(\|A'\|_{\HS}^2+\tr(K^2\rho)-\tr(\rho^q)\bigr)\,dx. \tag{3.1}

For pointwise matrix values A\in\R^{n\times d} and B\in\Sym_n, put

\Phi_K(A,B)=\min\left\{1, \|[B,K^2]\|_{\op}^2 +\|K^2-B^2-(AA^{\mathsf T})^r\|_{\op}^2\right\}. \tag{3.2}

Thus \Phi_K=0 expresses two algebraic relations, while A'-BA=0 is a first-order differential relation.

Theorem 3.1 (Quantitative finite-interval action estimate). Let 0<\sigma<1 and \kappa>0. There is a constant c_*=c_*(\sigma,\kappa)>0 with the following property. For n,d,\Omega,K as above, suppose U\in H^1_0(\Omega;\R^{n\times d}) satisfies

\int_\Omega UU^{\mathsf T}\,dx=I_n.

For every \eta>0 there exist a real lower triangular matrix C\in\R^{n\times n} and a path B\in C^1(\overline\Omega;\Sym_n) such that

B(x_-)=K,\qquad B(x_+)=-K,\qquad \sup_{x\in\overline\Omega}\|B(x)\|_{\op}\leq\kappa,

and, for A=CU,

\mathcal E_K(A)\geq b_\sigma\sum_{i=1}^n\ell_i^{2\gamma} +\int_\Omega\left(\|A'-BA\|_{\HS}^2 +c_*\Phi_K(A,B)\right)\,dx-\eta. \tag{3.3}

In particular, c_* is independent of n,d,\Omega,U, and the smallest diagonal entry of K.

3.1 Coercivity at the matrix-field constraint

The algebraic relations \Phi_K(A,B)=0 require [B,K^2]=0 and \rho=(K^2-B^2)^\sigma. For 0<\delta\leq1, we use a locally Lipschitz field M_\delta:\Sym_n\to\Sym_n extending the commuting rule

M_\delta(B)=(K^2-B^2+\delta I)^\sigma-\delta^\sigma I \quad\text{if }[B,K^2]=0\text{ and }K^2-B^2\geq0.

Thus the constraint M_\delta(B)=\rho is a regularized form of the algebraic equality relation in this case. The extension to arbitrary symmetric B has a C^1 primitive J_\delta:\Sym_n\to\R satisfying

dJ_\delta(B)[H]=-\tr(M_\delta(B)H). \tag{3.4}

Proposition B.1 constructs these maps and proves their required properties. Along a path B, the derivative identity converts -\tr(M_\delta(B)B') into the total derivative of J_\delta(B), which will supply the boundary term in the action identity. Its endpoint difference is explicit:

\begin{align*} J_\delta(-K)-J_\delta(K) &=\sum_{i=1}^n\int_{-\ell_i}^{\ell_i} \bigl((\ell_i^2-s^2+\delta)^\sigma-\delta^\sigma\bigr)\,ds \\ &\longrightarrow b_\sigma\sum_{i=1}^n\ell_i^{2\gamma} \qquad(\delta\downarrow0). \tag{3.5}\end{align*}

The limit follows by dominated convergence and 2\sigma+1=2\gamma.

Define the scalar function

F(A,B)=\tr(\rho^q)-\tr\bigl((K^2-B^2)\rho\bigr), \qquad \rho=AA^{\mathsf T}. \tag{3.6}

The following lemma bounds this nonlinear term while keeping the algebraic defect. The constraint in its hypothesis will later be enforced by a penalty.

Lemma 3.2. The constant c_*(\sigma,\kappa)>0 can be chosen so that, whenever 0<\delta\leq1, \|B\|_{\op}\leq\kappa, and M_\delta(B)=AA^{\mathsf T}, one has

F(A,B)+c_*\Phi_K(A,B)\leq E_{n,\delta}, \qquad E_{n,\delta} =n\bigl(\delta\kappa^{2\sigma} +\delta^\sigma(\kappa^2+\delta)\bigr) +\delta^{2\sigma}. \tag{3.7}

Proof. Write \rho=M_\delta(B)\geq0. Proposition B.2 gives

Q_s:=s^2I-2sB+K^2\geq0\quad(s\in\R), \qquad 0\leq\rho\leq\kappa^{2\sigma}I. \tag{3.8}

Put V=K^2-B^2+\delta I and \beta=\sigma-\tfrac12. With the positive normalization constant c_\sigma specified in (A.1), define

\begin{split} R(t)&=\frac1\pi\int_\R \bigl(Q_s+(\delta+t)I\bigr)^{-1}\,ds,\qquad t>0,\\ N&=c_\sigma\int_0^\infty t^\beta\bigl(t^{-1/2}I-R(t)\bigr)\,dt =\rho+\delta^\sigma I. \end{split} \tag{3.9}

The last identity is also part of Proposition B.2. Since (sI-B)^2+V=Q_s+\delta I\geq\delta I and N\geq0, Theorem A.1 applies. It supplies L(t)=R(t)^{-1}>0 and Hermitian matrices Z(t) satisfying

V+tI=L^2+Z^2+i[B,Z],\qquad LZ+ZL+i[B,L]=0, \tag{3.10}

and the exact identity

\begin{align*} \Delta&:=\tr(NV)-\tr(N^q)\\ &=c_\sigma\int_0^\infty t^\beta \left(\tr(R(t)Z(t)^2) +q\bigl\|R(t)^{-1/2} -R(t)^{1/2}(tI+N^r)^{1/2}\bigr\|_{\HS}^2\right)\,dt \geq0. \tag{3.11}\end{align*}

The matrices in (3.10) may be complex Hermitian even though A and B are real; i denotes the imaginary unit.

We extract a dimension-independent bound from the part of the integral with 1\leq t\leq2. On this interval there are constants a_\kappa,A_\kappa>0 such that

a_\kappa I\leq R(t)\leq A_\kappa I. \tag{3.12}

For the upper bound, use Q_s\geq0 on a bounded interval in s, and Q_s\geq\tfrac12s^2I for |s|\geq\max\{1,4\kappa\}. For the lower bound, restrict the integral to |s|\leq1, where Q_s+(\delta+t)I\leq(4+2\kappa+\kappa^2)I. These estimates depend on \kappa alone. Moreover \|N\|_{\op}\leq\kappa^{2\sigma}+1, so H_t=(tI+N^r)^{1/2} and L(t) are bounded in operator norm by constants depending only on \sigma,\kappa.

The two integrands in (3.11) control \|Z(t)\|_{\HS}^2 and \|L(t)-H_t\|_{\HS}^2: indeed \tr(RZ^2)=\tr(ZRZ) and

R^{-1/2}-R^{1/2}H_t=R^{1/2}(L-H_t).

It follows by averaging over [1,2] that at some t in this interval,

\|Z(t)\|_{\op}+\|L(t)-H_t\|_{\op} \leq C_1\sqrt\Delta, \tag{3.13}

where C_1 depends only on \sigma,\kappa. When \Delta=0, the same conclusion follows by taking a point where both nonnegative integrands vanish.

Suppose first that \Delta\leq1, and use this value of t. The first identity in (3.10) gives

V-N^r=(L^2-H_t^2)+Z^2+i[B,Z].

The boundedness of L,H_t,B, together with (3.13), bounds the norm of this expression by C_2\sqrt\Delta. To control the commutator, the second identity in (3.10) first yields \|[B,L]\|_{\op}\leq2\|L\|_{\op}\|Z\|_{\op}. Then

[B,V]=[B,L^2]+[B,Z^2]+i[B,[B,Z]]

has the same bound. Thus

\|V-N^r\|_{\op}+\|[B,V]\|_{\op} \leq C_3\sqrt\Delta. \tag{3.14}

Here and below the constants in this proof depend only on \sigma,\kappa.

The matrices N=\rho+\delta^\sigma I and \rho commute. Because r>1, the scalar function y\mapsto y^r is Lipschitz on [0,\kappa^{2\sigma}+1]. Consequently

\|N^r-\rho^r\|_{\op}\leq C_4\delta^\sigma.

Since [B,V]=[B,K^2] and \delta\leq\delta^\sigma, (3.14) implies

\|[B,K^2]\|_{\op}^2 +\|K^2-B^2-\rho^r\|_{\op}^2 \leq C_5(\Delta+\delta^{2\sigma}).

Choose c_*>0 sufficiently small, also with c_*\leq1. For \Delta\leq1 the preceding estimate gives

c_*\Phi_K(A,B)\leq\Delta+\delta^{2\sigma}. \tag{3.15}

For \Delta>1 this follows directly from \Phi_K\leq1. This proves the required uniform control of the algebraic defect.

It remains to relate \Delta to F. Expanding N and V gives

F(A,B)=-\Delta+\tr(\rho^q)-\tr(N^q) +\delta\tr\rho+\delta^\sigma\tr V.

The first two powers are ordered because N=\rho+\delta^\sigma I. Also \tr\rho\leq n\kappa^{2\sigma} and V\leq(\kappa^2+\delta)I. Adding (3.15) now proves (3.7).

3.2 The action identity and the penalty limit

Proof of Theorem 3.1. Fix 0<\delta\leq1. Proposition B.3 supplies, for every 0<\varepsilon\leq1, a lower triangular matrix C_\varepsilon and a path B_\varepsilon with the prescribed endpoints and operator-norm bound such that, for A_\varepsilon=C_\varepsilon U,

\varepsilon B_\varepsilon' =M_\delta(B_\varepsilon) -A_\varepsilon A_\varepsilon^{\mathsf T}. \tag{3.16}

For fixed \delta,K,\Omega,U, the matrices C_\varepsilon are bounded uniformly in 0<\varepsilon\leq1.

Temporarily suppress the subscript \varepsilon and write

u_\delta(A,B) =\|M_\delta(B)-AA^{\mathsf T}\|_{\HS}^2.

Since A\in H^1_0 and B\in C^1, the product and chain rules for absolutely continuous functions, (3.4), and (3.16) yield almost everywhere

\begin{align*} \bigl(J_\delta(B)+\tr(A^{\mathsf T}BA)\bigr)' &=2\tr((A')^{\mathsf T}BA) -\tr\bigl((M_\delta(B)-AA^{\mathsf T})B'\bigr)\\ &=2\tr((A')^{\mathsf T}BA)-\varepsilon^{-1}u_\delta(A,B).\end{align*}

Complete the square in the action and integrate this identity. Because A vanishes at both endpoints, the result is the exact formula

\begin{align*} \mathcal E_K(A) &=J_\delta(-K)-J_\delta(K)\\ &\quad+\int_\Omega\left( \|A'-BA\|_{\HS}^2-F(A,B) +\varepsilon^{-1}u_\delta(A,B)\right)\,dx. \tag{3.17}\end{align*}

We now use the penalty to pass from the constraint estimate in Lemma 3.2 to all matrix values on these paths. The continuous representative of U is bounded on \overline\Omega. The uniform bound on C_\varepsilon and the bound \|B_\varepsilon\|_{\op}\leq\kappa therefore place all pairs (A_\varepsilon(x),B_\varepsilon(x)) in one compact set \mathcal K_\delta\subset\R^{n\times d}\times\Sym_n on which \|B\|_{\op}\leq\kappa. On this set F, \Phi_K, and u_\delta are continuous. Lemma 3.2 implies

\limsup_{\varepsilon\downarrow0} \sup_{(A,B)\in\mathcal K_\delta} \bigl(F(A,B)+c_*\Phi_K(A,B)-\varepsilon^{-1}u_\delta(A,B)\bigr) \leq E_{n,\delta}. \tag{3.18}

Indeed, if the left side exceeded E_{n,\delta}, some sequence \varepsilon_j\downarrow0 and corresponding pairs in the compact set would make the expression at least E_{n,\delta}+\tau for some \tau>0. Boundedness of F+c_*\Phi_K would force u_\delta=O(\varepsilon_j) along that sequence. A convergent subsequence would then give a limiting pair with u_\delta=0 and F+c_*\Phi_K\geq E_{n,\delta}+\tau, contradicting Lemma 3.2.

For any \tau>0, choose \varepsilon small enough that the supremum in (3.18) is at most E_{n,\delta}+\tau. Substitution into (3.17) gives

\begin{align*} \mathcal E_K(A_\varepsilon) \geq{}&J_\delta(-K)-J_\delta(K) -|\Omega|(E_{n,\delta}+\tau)\\ &+\int_\Omega\left(\|A_\varepsilon'-B_\varepsilon A_\varepsilon\|_{\HS}^2 +c_*\Phi_K(A_\varepsilon,B_\varepsilon)\right)\,dx.\end{align*}

Finally, first choose \delta>0 so small that the endpoint error in (3.5) and |\Omega|E_{n,\delta} together are less than \eta/2. Next choose \tau>0 with |\Omega|\tau<\eta/2, and then choose the required \varepsilon. These choices prove (3.3). All compactness arguments were made after fixing \delta; no bound uniform in \delta is needed.

4 Recovering the sharp spectral bound

The action estimate implies the sharp inequality by the spectral passage of [11, Section 7]. We record it before studying equality, so that the finite spectral moment used below has already been established.

Proposition 4.1. Every potential in Theorem 1.1 satisfies

\Tr(H_W)_-^\gamma\le\frac{D_\sigma}{b_\sigma} \int_\R\tr(W^p).

Proof. First suppose that W is real symmetric. Choose any finite initial list of negative eigenvalues -k_1^2,\ldots,-k_n^2, with k_1\ge\cdots\ge k_n>0, and real orthonormal eigenfunctions \varphi_i. For 0<\xi<k_n^2 put \ell_i=(k_i^2-\xi)^{1/2} and K=\diag(\ell_1,\ldots,\ell_n). There are real smooth compactly supported orthonormal functions u_i with form matrix

(h_W[u_i,u_j])_{i,j=1}^n\le-K^2. \tag{4.1}

Indeed, approximate the \varphi_i in H^1, then multiply the family by the inverse square root of its Gram matrix. The Gram matrix tends to I_n, and the form matrix tends to -\diag(k_i^2) by Lemma 2.1; an operator norm error below \xi gives (4.1).

Let U have rows u_i, and choose a bounded interval containing their supports. For every lower triangular C, the ith row a_i of A=CU satisfies

h_W[a_i]+\ell_i^2\|a_i\|_2^2 \le\sum_{l\le i}C_{il}^2(\ell_i^2-\ell_l^2)\le0.

Set Z=A^TA. The matrices AA^T and Z have the same nonzero eigenvalues, with multiplicity. Summing the preceding bound and applying Lemma 2.2 yields

\mathcal E_K(A) \le\int_\R\{\tr(WZ)-\tr(Z^q)\} \le D_\sigma\int_\R\tr(W^p).

Theorem 3.1, with its nonnegative defects discarded, gives b_\sigma\sum_i\ell_i^{2\gamma}\le D_\sigma\int\tr(W^p)+\eta for every \eta>0. Let \eta\downarrow0, then \xi\downarrow0, and finally exhaust the negative eigenvalues. The case of an empty negative spectrum is immediate.

For complex Hermitian W=E+iF, with E,F real, its realification is

\widetilde W=\begin{pmatrix}E&-F\\F&E\end{pmatrix}. \tag{4.2}

The constant unitary matrix 2^{-1/2}\left(\begin{smallmatrix}I&iI\\I&-iI\end{smallmatrix}\right) conjugates \widetilde W to W\oplus\overline W. Hence \widetilde W is real symmetric and positive semidefinite, \tr(\widetilde W^p)=2\tr(W^p), and \Tr(H_{\widetilde W})_-^\gamma=2\Tr(H_W)_-^\gamma. Here conjugation identifies the spectra of H_W and H_{\overline W}. The real inequality, divided by two, proves the result.

5 From equality to pointwise matrix relations

We now apply Theorem 3.1 to finite collections of negative eigenfunctions. Equality forces each of its nonnegative errors to vanish. The main issue is that the number of eigenfunctions may grow without bound, whereas the potential has only m channels. We will use this fixed number of columns to control the tails of the resulting matrices.

Throughout this section, W is real symmetric, W\geq0 almost everywhere, and 0<\int_{\R}\tr(W^p)<\infty. Suppose that equality holds, in the form

b_\sigma\sum_{i\in\mathcal I}k_i^{2\gamma} =D_\sigma\int_{\R}\tr(W^p)\,dx, \tag{5.1}

where -k_i^2 are the negative eigenvalues of H_W, repeated according to multiplicity, and

k_1\geq k_2\geq\cdots>0.

By Lemma 2.1, the index set \mathcal I is a nonempty finite initial segment of \mathbb N or all of \mathbb N, each eigenvalue has finite multiplicity, and k_i\to0 in the infinite case. Fix real orthonormal eigenfunctions \varphi_i\in H^1(\R;\R^m) and regard them as row vectors. Write

\mathscr H=\ell^2(\mathcal I;\R),\qquad \Lambda=\operatorname{diag}(k_i:i\in\mathcal I),\qquad \kappa=k_1.

For operators between real Hilbert spaces, the superscript T will also denote the adjoint.

Proposition 5.1 (Pointwise relations at equality). Under these assumptions, there are rows a_i\in H^1(\R;\R^m), i\in\mathcal I, each a linear combination of eigenfunctions with eigenvalue -k_i^2, such that

-a_i''-a_iW=-k_i^2a_i \quad\text{in distributions.} \tag{5.2}

The rows a_i are allowed to vanish. On a common set of full measure, they define a Hilbert–Schmidt operator A(x):\R^m\to\mathscr H, and there exists a bounded self-adjoint operator B on \mathscr H with \|B\|_{\op}\leq\kappa such that

[B,\Lambda^2]=0,\qquad \Lambda^2-B^2=(AA^T)^r,\qquad a_i'(x)=(BA)_{i,\cdot}\quad(i\in\mathcal I). \tag{5.3}

Moreover,

W(x)=q\bigl(A(x)^TA(x)\bigr)^r \quad\text{almost everywhere.} \tag{5.4}

The operator B is asserted to exist separately at each such point x; no measurable choice is required.

We divide the proof into the construction of a sequence whose errors vanish, convergence of every fixed row, and control of the remaining rows.

5.1 Finite spectral approximations and vanishing errors

Let n_j=j when \mathcal I=\mathbb N, and let n_j=|\mathcal I| when \mathcal I is finite. Choose 0<\xi_j<1/j so small that

\ell_{j,i}:=(k_i^2-\xi_j)^{1/2}>0\quad(1\leq i\leq n_j), \qquad \sum_{i\leq n_j}\bigl(k_i^{2\gamma}-\ell_{j,i}^{2\gamma}\bigr)<1/j. \tag{5.5}

Set K_j=\operatorname{diag}(\ell_{j,1},\ldots,\ell_{j,n_j}). The same shift \xi_j is used for every eigenvalue: this leaves the differences of their squares unchanged.

The approximation leading to (4.1) can be made arbitrarily accurate in H^1. Apply it to the first n_j eigenfunctions, choosing the H^1 errors below 1/j and the form-matrix error below \xi_j. This gives real, smooth, compactly supported functions u_{j,1},\ldots,u_{j,n_j}, orthonormal in L^2(\R;\R^m), such that

\|u_{j,i}-\varphi_i\|_{H^1}<1/j, \qquad \bigl(h_W[u_{j,i},u_{j,l}]\bigr)_{i,l=1}^{n_j}\leq-K_j^2. \tag{5.6}

Here h_W[\cdot,\cdot] is the polarized quadratic form, and the second inequality is the ordering of real symmetric matrices.

Let U_j be the matrix with rows u_{j,i}, and choose a bounded interval \Omega_j containing their supports in its interior. Apply Theorem 3.1 with K=K_j, d=m, \kappa=k_1, and \eta=1/j. It gives a lower triangular matrix C_j, a symmetric path B_j with \|B_j\|_{\op}\leq\kappa, and A_j=C_jU_j. Extend A_j by zero outside \Omega_j and extend B_j by K_j to the left and by -K_j to the right. All the errors in that theorem vanish outside \Omega_j, so their integrals may be taken over \R.

The lower triangular form of C_j gives a useful additional error. Put Z_j=A_j^TA_j, an m\times m positive semidefinite matrix. By (5.6),

\mathcal E_{K_j}(A_j) \leq\int_{\R}\bigl(\tr(WZ_j)-\tr(Z_j^q)\bigr)\,dx-T_j, \qquad T_j=\sum_{l\leq i\leq n_j}(C_j)_{il}^{\,2}(k_l^2-k_i^2)\geq0. \tag{5.7}

Indeed, the ith row of A_j is \sum_{l\leq i}(C_j)_{il}u_{j,l}. Its quadratic form, plus \ell_{j,i}^2 times its squared L^2 norm, is at most

\sum_{l\leq i}(C_j)_{il}^{\,2} (\ell_{j,i}^2-\ell_{j,l}^2) =-\sum_{l\leq i}(C_j)_{il}^{\,2}(k_l^2-k_i^2).

Summing over i proves (5.7), since A_jA_j^T and Z_j have the same nonzero eigenvalues, with multiplicity. The ordering of the k_i makes every summand of T_j nonnegative.

Recall the nonnegative Young deficit from Lemma 2.2:

Y(W,Z)=D_\sigma\tr(W^p)-\tr(WZ)+\tr(Z^q)\geq0, \qquad Y(W,Z)=0\ \Longleftrightarrow\ W=qZ^r. \tag{5.8}

Combining Theorem 3.1, (5.1), and (5.7) yields

\begin{align*} 0\leq T_j+\int_{\R}\Bigl( Y(W,Z_j)+\|A_j'-B_jA_j\|_{\HS}^2 +c_*\Phi_{K_j}(A_j,B_j)\Bigr)\,dx &\leq d_j,\tag{5.9}\\ d_j:=b_\sigma\left( \sum_{i\in\mathcal I}k_i^{2\gamma} -\sum_{i\leq n_j}\ell_{j,i}^{2\gamma}\right)+1/j &\longrightarrow0.\end{align*}

Here c_*>0 is fixed: its independence of n_j is essential. Thus all three integral errors tend to zero, as does T_j.

We will also need a uniform bound on A_j. The coercive estimate (2.3) gives

Y(W,Z_j)\geq\frac12\tr(Z_j^q) -(2^{p-1}-1)D_\sigma\tr(W^p). \tag{5.10}

Since Z_j has size m, scalar Hölder’s inequality gives

\|A_j\|_{\HS}^{2q}=(\tr Z_j)^q \leq m^{q-1}\tr(Z_j^q).

Equations (5.9) and (5.10) therefore bound A_j uniformly in L^{2q}(\R) with the Hilbert–Schmidt norm, independently of its number of rows.

5.2 Convergence of each fixed row

For fixed i\in\mathcal I, the coefficients (C_j)_{il}, l\leq i, are bounded as j\to\infty. To see this, choose a bounded interval J_i so large that the restricted Gram matrix

\left(\int_{J_i}\varphi_l(x)\varphi_s(x)^T\,dx \right)_{l,s=1}^{i}\geq\frac34 I_i,

where I_i denotes the i\times i identity matrix. Such an interval exists because the full Gram matrix is the identity. By (5.6), the corresponding restricted Gram matrix of the u_{j,l} is at least one half of the identity for all sufficiently large j. Hence

\frac12\sum_{l\leq i}(C_j)_{il}^{\,2} \leq\int_{J_i}|(A_j)_{i,\cdot}|^2\,dx \leq |J_i|^{1-1/q} \left(\int_{J_i}\|A_j\|_{\HS}^{2q}\,dx\right)^{1/q}.

The last expression is uniformly bounded. Lower triangularity is used here to keep the number of coefficients in a fixed row finite.

A diagonal subsequence now makes every coefficient (C_j)_{il} converge to a limit c_{il}, for l\leq i. From T_j\to0 and (5.7),

c_{il}=0\quad\text{whenever }k_l>k_i. \tag{5.11}

Define

a_i=\sum_{l\leq i}c_{il}\varphi_l.

The sum is finite, and (5.6) implies

(A_j)_{i,\cdot}\longrightarrow a_i \quad\text{in }H^1(\R;\R^m) \quad\text{for every fixed }i. \tag{5.12}

The ordering of the eigenvalues and (5.11) show that only eigenfunctions with eigenvalue -k_i^2 occur in a_i. This proves (5.2), including the possibility a_i=0. The eigenfunction equations hold distributionally by testing the form equations against smooth compactly supported functions; the potential is locally integrable and the rows are locally bounded.

Choose the continuous, locally absolutely continuous representatives of these rows. The Sobolev embedding H^1(\R)\subset C_b(\R) shows that (5.12) also gives pointwise convergence at every x. Passing to a further subsequence, we may arrange that the integrals of the nonnegative integrand in (5.9) are summable, and that, for every fixed i, the squared L^2 errors of the derivatives in (5.12) are summable. A diagonal choice achieves both conditions, by making the first j available derivative errors and the integral error less than 2^{-j} along the chosen subsequence. Consequently, on a common set of full measure,

\begin{gathered} Y(W,Z_j)\to0,\qquad \|A_j'-B_jA_j\|_{\HS}\to0,\qquad \Phi_{K_j}(A_j,B_j)\to0,\\ (A_j')_{i,\cdot}(x)\to a_i'(x) \quad\text{for every }i\in\mathcal I. \end{gathered} \tag{5.13}

We also exclude the null set where W is not a finite positive semidefinite matrix. It remains to show that convergence of the individual rows is strong enough to pass to the products in these relations.

5.3 Tail control in the row-index space

Pad A_j, B_j, and K_j with zeros in the unused coordinates of \mathscr H. Thus A_j:\R^m\to\mathscr H, and B_j,K_j are self-adjoint finite-rank operators on \mathscr H. Since the omitted k_i tend to zero,

\|K_j^2-\Lambda^2\|_{\op} \leq\max\{\xi_j,\sup_{i>n_j}k_i^2\}\longrightarrow0, \tag{5.14}

where a supremum over no indices is zero.

Fix a point x in the full-measure set from (5.13) and suppress x for the moment. Write \rho_j=A_jA_j^T. The definition of \Phi and its convergence to zero give

\|[B_j,K_j^2]\|_{\op}\to0, \qquad e_j:=\|K_j^2-B_j^2-\rho_j^r\|_{\op}\to0. \tag{5.15}

For h\geq1, let P_h be the orthogonal projection onto the first h coordinates of \mathscr H, with all coordinates included if h exceeds |\mathcal I|. Set Q_h=I-P_h and s_h=\sup_{i>h}k_i^2, again with the empty supremum equal to zero. Then s_h\to0. For every unit vector v in the range of Q_h,

\|B_jv\|^2+\langle v,\rho_j^rv\rangle\leq s_h+e_j. \tag{5.16}

Both terms on the left are nonnegative. Jensen’s inequality for the spectral measure of \rho_j, using r>1, implies

\langle v,\rho_jv\rangle^r\leq\langle v,\rho_j^rv\rangle.

It follows that \|Q_h\rho_jQ_h\|_{\op}\leq(s_h+e_j)^{1/r}. Although \mathscr H may be infinite dimensional, Q_h\rho_jQ_h has rank at most m, because A_j has exactly m columns. Its trace is therefore at most m times its operator norm. We obtain the two tail bounds

\boxed{\quad \|Q_hA_j\|_{\HS}^2\leq m(s_h+e_j)^{1/r}, \qquad \|B_jQ_h\|_{\op}\leq(s_h+e_j)^{1/2}. \quad} \tag{5.17}

The first estimate converts decay of the eigenvalue parameters into decay of the total mass of all omitted rows. Its factor is the fixed physical dimension m, rather than the number of retained eigenfunctions; Figure 1 depicts this distinction.

Figure 1: The number of rows can grow with the number of negative eigenfunctions, but the number of physical channels remains m. After fixing the first h rows, the identity K_j^2\approx B_j^2+(A_jA_j^T)^r bounds the operator norm in the remaining rows. The rank bound converts it into a Hilbert–Schmidt bound, which tends to zero as first j\to\infty and then h\to\infty. The drawing is schematic; all matrices are padded by zero rows in \mathscr H.

For each fixed h, the first h rows of A_j converge by (5.12). The first bound in (5.17) makes the remaining rows uniformly small by choosing h large and then j sufficiently large. Thus A_j is Cauchy in Hilbert–Schmidt norm and converges to an operator A:\R^m\to\mathscr H whose rows are precisely a_i(x):

A_j\longrightarrow A\quad\text{in Hilbert--Schmidt norm.} \tag{5.18}

This argument applies to the whole subsequence already selected and does not require a further choice depending on x.

For B_j we need only pointwise compactness. Its finite compressions P_hB_jP_h are bounded in finite-dimensional spaces, so a diagonal subsequence makes them converge for every h. Self-adjointness and the second estimate in (5.17) give

\|B_j-P_hB_jP_h\|_{\op} \leq2\|B_jQ_h\|_{\op} \leq2(s_h+e_j)^{1/2}.

The chosen subsequence consequently converges in operator norm to a self-adjoint B with \|B\|_{\op}\leq\kappa. This subsequence, and hence B, may depend on the point x.

We can now pass to all the required products. Hilbert–Schmidt convergence of A_j implies operator norm convergence of A_jA_j^T and of A_j^TA_j. Continuous functional calculus for nonnegative operators then gives convergence of their rth powers. Together with (5.14) and (5.15), this proves

[B,\Lambda^2]=0,\qquad \Lambda^2-B^2=(AA^T)^r.

Also B_jA_j\to BA in Hilbert–Schmidt norm. Taking its ith row and using both the derivative convergence and the first-order error in (5.13) gives a_i'(x)=(BA)_{i,\cdot} for every i. Finally, continuity of the finite-dimensional Young deficit and Y(W,A_j^TA_j)\to0 yield Y(W,A^TA)=0. Lemma 2.2 gives W=q(A^TA)^r.

We have proved these statements at every point of one common set of full measure. The construction selects no function x\mapsto B(x): only the existence of a suitable operator at each such point enters the next section. This completes the proof of Proposition 5.1.

6 Fixed channels and the equality profiles

The pointwise relations of Proposition 5.1 still involve an auxiliary operator B that may depend on the point without a prescribed measurable choice. We now extract constant subspaces from those relations. On each nonzero subspace, B becomes a uniquely determined matrix and satisfies an ordinary differential equation. This will identify every real equality potential; realification and a scalar calculation will then complete the proof of Theorem 1.1.

6.1 The channel subspaces are constant

Assume first that W is real and is a nonzero equality potential. Use the rows a_i, numbers k_i, and operator \Lambda=\operatorname{diag}(k_i) from Proposition 5.1. For each distinct value \alpha>0 in the list (k_i), let n_\alpha be its finite multiplicity, and let G_\alpha be the n_\alpha\times m matrix whose rows are the a_i with k_i=\alpha. Each G_\alpha has entries in H^1(\R), and we use their continuous representatives.

At every point in the common full-measure set of that proposition, choose one of the operators B it supplies. Since B commutes with \Lambda^2, it preserves each of its eigenspaces. Moreover,

AA^T=(\Lambda^2-B^2)^{1/r}

commutes with both B and \Lambda^2. Writing B_\alpha for the block on the \alpha^2-eigenspace therefore gives

\begin{align*} G_\alpha G_\beta^T&=0 &&(\alpha\ne\beta), \tag{6.1}\\ G_\alpha'&=B_\alpha G_\alpha, & [B_\alpha,G_\alpha G_\alpha^T]&=0, \tag{6.2}\\ \alpha^2I-B_\alpha^2&=(G_\alpha G_\alpha^T)^r, &\|B_\alpha\|_{\op}&\le\kappa. \tag{6.3}\end{align*}

These statements hold almost everywhere and require no compatibility between the choices of B at different points.

Lemma 6.1. For every \alpha, the subspace

\mathcal R_\alpha=(\ker G_\alpha(x))^\perp\subset\R^m

is independent of x\in\R. The nonzero spaces \mathcal R_\alpha are mutually orthogonal, and

\sum_\alpha\dim\mathcal R_\alpha\le m. \tag{6.4}

In particular, only finitely many G_\alpha are nonzero. The potential W has a continuous representative, equal to zero on the orthogonal complement of these spaces and equal to q(G_\alpha^TG_\alpha)^r on \mathcal R_\alpha. With this representative, every G_\alpha is C^2.

Proof. Fix v\in\R^m. Equation (6.2) implies

\|(G_\alpha v)'(x)\|\le\kappa\|G_\alpha(x)v\| \quad\text{for almost every }x.

The function G_\alpha v is locally absolutely continuous. If it vanishes at x_0, integration and Gronwall’s inequality, first to the right and then to the left of x_0, show that it vanishes everywhere. Consequently \ker G_\alpha(x) is independent of x, including points outside the original full-measure set. This proves the first assertion.

The products in (6.1) are continuous, so their almost-everywhere vanishing implies their vanishing everywhere. Thus the constant row spaces \mathcal R_\alpha are mutually orthogonal. Any finite collection has total dimension at most m, proving (6.4) and finiteness of the nonzero blocks.

On the full-measure set from Proposition 5.1, A^TA=\sum_\alpha G_\alpha^TG_\alpha. Each summand acts on its own orthogonal space \mathcal R_\alpha, and only finitely many summands are nonzero. Equation (5.4) therefore yields

W=q\sum_\alpha(G_\alpha^TG_\alpha)^r \quad\text{almost everywhere}. \tag{6.5}

The right-hand side is continuous and has the asserted restrictions; we henceforth use it as the representative of W. The row eigenfunction equation (5.2) now reads

G_\alpha''=\alpha^2G_\alpha-G_\alpha W \quad\text{in distributions}. \tag{6.6}

Its right-hand side is continuous. Integrating this identity twice shows that the continuous representative of G_\alpha is C^2.

The row spaces already split the physical space \R^m into finitely many constant channels. To determine the potential within one of them, we also need a constant range for G_\alpha in the eigenfunction index space \R^{n_\alpha}.

Lemma 6.2. For each \alpha with \ell:=\dim\mathcal R_\alpha>0, the range of G_\alpha(x) in \R^{n_\alpha} is independent of x. In constant orthonormal bases of this range and of \mathcal R_\alpha, the restriction of G_\alpha is an invertible C^2 matrix D:\R\to\R^{\ell\times\ell}. The matrix B_0=D'D^{-1} is C^1 and satisfies, everywhere on \R,

B_0=B_0^T,\qquad \alpha^2I-B_0^2=(DD^T)^r>0,\qquad B_0'=r(B_0^2-\alpha^2I). \tag{6.7}

Proof. Choose a constant orthonormal basis of \mathcal R_\alpha, and let E(x) be the matrix of the restriction of G_\alpha(x) to this space. It has full column rank \ell at every point, since the kernel of G_\alpha is constant. The projection onto its range is

P(x)=E(x)(E(x)^TE(x))^{-1}E(x)^T.

The commutator in (6.2) shows that B_\alpha preserves the range of G_\alpha G_\alpha^T, which is precisely the range of E. Hence E'=B_\alpha E has its columns in this range almost everywhere. Differentiating the projection gives

\begin{align*} P'={}&(I-P)E'(E^TE)^{-1}E^T\\ &+E(E^TE)^{-1}(E')^T(I-P)=0 \quad\text{almost everywhere}.\end{align*}

Since P is C^1, it is constant.

Choose a constant orthonormal basis of this range as well. The resulting square matrix D is invertible everywhere and C^2. Almost everywhere, D'D^{-1} is the restriction of B_\alpha to its invariant range in these coordinates. Equations (6.2) and (6.3) give the symmetry and square identity in (6.7) almost everywhere; continuity extends them to every point. Positivity is strict because D is invertible.

On \mathcal R_\alpha, Equation (6.5) identifies the potential with q(D^TD)^r. Equation  (6.6) consequently becomes

D''=\alpha^2D-qD(D^TD)^r =\alpha^2D-q(DD^T)^rD.

The second equality follows, for example, by a singular-value decomposition. Differentiating B_0=D'D^{-1} and using q=r+1 now gives

B_0'=D''D^{-1}-B_0^2 =\alpha^2I-q(\alpha^2I-B_0^2)-B_0^2 =r(B_0^2-\alpha^2I),

as claimed.

6.2 The matrix Riccati equation separates the profiles

Fix a nonzero block and the matrices of Lemma 6.2. Diagonalize the symmetric matrix B_0(x_*) at one point by a constant orthogonal change of range coordinates. The right-hand side of its Riccati equation is a polynomial in B_0. Uniqueness for this matrix ordinary differential equation therefore preserves the diagonal form. More explicitly, the strict inequality in (6.7) places each initial diagonal entry in (-\alpha,\alpha). There is a unique y_j\in\R such that the scalar solution with that initial value is

b_j(x)=-\alpha\tanh\bigl(r\alpha(x-y_j)\bigr), \qquad 1\le j\le\ell. \tag{6.8}

The diagonal matrix with these entries solves the same initial-value problem as B_0 on all of \R, so uniqueness gives equality everywhere.

Equation (6.7) implies that DD^T is diagonal in these coordinates. Since D'=\operatorname{diag}(b_j)D, each row of D is a positive scalar multiple of its value at x_*. None of these rows is zero, and their directions are mutually orthogonal because DD^T is diagonal. Taking their normalized directions as a constant orthonormal basis of \mathcal R_\alpha makes D diagonal with positive entries. The potential in this fixed basis is therefore diagonal, with entries

q\bigl(\alpha^2-b_j(x)^2\bigr) =(r+1)\alpha^2\operatorname{sech}^2\bigl(r\alpha(x-y_j)\bigr). \tag{6.9}

Combining these bases over the finitely many nonzero spaces \mathcal R_\alpha, and adding a basis of their orthogonal complement, proves the required necessity for real W. There are at most m nonzero profiles by (6.4). The zero potential has the same description with no nonzero profile.

6.3 Complex Hermitian potentials

For a complex Hermitian potential W, take the realification \widetilde W from (4.2). The proof of Proposition 4.1 shows that it is equivalent to W\oplus\overline W by a constant unitary matrix and that both the trace-power integral and the negative spectral moment are doubled. Thus equality for W implies equality for the real potential \widetilde W.

The real result provides a constant unitary matrix V such that

W(x)\oplus\overline W(x) =V\operatorname{diag}(f_1(x),\ldots,f_{2m}(x))V^* \quad\text{almost everywhere},

where each f_j is either a profile of the form (6.9) or zero. Let P be the projection onto the first summand \C^m and put \widehat P=V^*PV. Since P commutes with W\oplus\overline W,

(f_i(x)-f_j(x))\widehat P_{ij}=0 \quad\text{almost everywhere}.

Consequently \widehat P_{ij}=0 whenever the functions f_i,f_j are not equal almost everywhere. Partition the indices into groups of identical functions, including the possible zero function. The range of \widehat P splits as the orthogonal sum of its intersections with these coordinate groups. On each group the diagonal potential is a scalar multiple of the identity, so any constant orthonormal basis of that intersection diagonalizes its restriction. Transporting these bases by V to the first summand gives a constant unitary basis of \C^m in which W has the asserted profiles. This proves necessity for complex Hermitian potentials.

6.4 Each listed potential attains equality

It remains to verify attainment, including the exact spectral moment, without appealing to a classification of scalar optimizers. Fix a>0 and x_0\in\R, and set

V(x)=(r+1)a^2\operatorname{sech}^2\bigl(ra(x-x_0)\bigr), \qquad H=-\partial_x^2-V.

The first-order factorization used in the commutation argument of [2, Section II] also explains why this profile has only one negative eigenvalue. Put

w(x)=a\tanh\bigl(ra(x-x_0)\bigr), \qquad Q=\partial_x+w,\qquad \operatorname{Dom}Q=H^1(\R).

Then Q^*=-\partial_x+w on H^1(\R). Since w and w' are bounded, both product domains are H^2(\R), and direct differentiation yields

\begin{align*} Q^*Q&=H+a^2, \tag{6.10}\\ QQ^*&=-\partial_x^2+a^2 +(r-1)a^2\operatorname{sech}^2\bigl(ra(x-x_0)\bigr) \ge a^2. \tag{6.11}\end{align*}

Here the last inequality uses r>1. The equation Q\psi=0 has the one-dimensional L^2 solution space

\ker Q= \operatorname{span}\left\{ \operatorname{sech}^{1/r}\bigl(ra(x-x_0)\bigr) \right\}.

Thus -a^2 is a simple eigenvalue of H, and (6.10) excludes eigenvalues below it. If H\phi=\lambda\phi with -a^2<\lambda<0, put \mu=\lambda+a^2 and g=Q\phi. Then \|g\|_2^2=\mu\|\phi\|_2^2>0. Moreover, Q^*Q\phi=\mu\phi\in\operatorname{Dom}Q, so g\in\operatorname{Dom}(QQ^*) and QQ^*g=\mu g. This contradicts (6.11), since \mu<a^2. By Lemma 2.1, all negative spectrum is discrete. Hence -a^2 is the sole negative eigenvalue.

Finally, 2p-1=2\gamma and the substitution s=\tanh y give

\begin{align*} \int_\R V(x)^p\,dx &=\frac{(r+1)^p}{r}a^{2\gamma} \int_\R\operatorname{sech}^{2p}y\,dy\\ &=\frac{(r+1)^p}{r}a^{2\gamma} \int_{-1}^{1}(1-s^2)^{p-1}\,ds =\frac{b_\sigma}{D_\sigma}a^{2\gamma},\end{align*}

where (r+1)^p/r=D_\sigma^{-1} and p-1=\sigma. Consequently

\operatorname{Tr}(H)_-^\gamma =a^{2\gamma} =C_\gamma\int_\R V^p.

The zero potential contributes zero to both sides. Finite orthogonal direct sums add the spectral moments and trace-power integrals, and a constant unitary conjugation leaves both unchanged. Every potential listed in Theorem 1.1 therefore attains equality, completing its proof.

A The exact integrated trace deficit

The matrix comparison needed in the action argument has an exact remainder. We give the proof from [11, Section 3], retaining both nonnegative terms. Together they control the commutator and the algebraic equality relation used in the action argument. Throughout this appendix, 0<\sigma<1, \beta=\sigma-\tfrac12, and r=1/\sigma, p=1+\sigma, q=1+r. Define c_\sigma>0 by

c_\sigma^{-1} =\int_0^\infty t^\beta \bigl(t^{-1/2}-(t+1)^{-1/2}\bigr)\,dt. \tag{A.1}

The integrand is O(t^{\sigma-1}) at zero and O(t^{\sigma-2}) at infinity. Scaling therefore gives

c_\sigma\int_0^\infty t^\beta \bigl(t^{-1/2}-(t+y)^{-1/2}\bigr)\,dt=y^\sigma, \qquad y\geq0. \tag{A.2}

Theorem A.1 (Exact trace deficit). Let n\geq1 and let B,V\in\C^{n\times n} be Hermitian. Suppose that

Y_s=(sI-B)^2,\qquad X_s=Y_s+V\geq bI \quad(s\in\R) \tag{A.3}

for some b>0. Set

R(t)=\frac1\pi\int_\R(X_s+tI)^{-1}\,ds, \qquad P(t)=t^{-1/2}I-R(t),\qquad t>0, \tag{A.4}

and

N=c_\sigma\int_0^\infty t^\beta P(t)\,dt. \tag{A.5}

These integrals converge absolutely in matrix norm, and R(t)>0. There are continuous Hermitian matrices L(t)=R(t)^{-1}>0 and Z(t) satisfying

V+tI=L^2+Z^2+i[B,Z],\qquad LZ+ZL+i[B,L]=0. \tag{A.6}

If N\geq0, then

\begin{split} \tr(NV)-\tr(N^q) =c_\sigma\int_0^\infty t^\beta\Bigl( \tr(RZ^2) +q\bigl\|R^{-1/2}-R^{1/2}(tI+N^r)^{1/2}\bigr\|_{\HS}^2 \Bigr)\,dt. \end{split} \tag{A.7}

In particular, \tr(NV)\geq\tr(N^q).

The hypothesis concerns the full symbol X_s; the perturbation V itself need not be positive. The proof first recovers L and Z from solutions on the two half-lines, then evaluates a logarithmic integral, and finally completes a matrix square.

A.1 Half-line boundary maps

Quadratic growth in s, together with (A.3), gives an integrable bound for X_s^{-1}. Hence R(t)>0 and R(t)=O(1) as t\downarrow0. Diagonalization of B gives

\frac1\pi\int_\R(Y_s+tI)^{-1}\,ds=t^{-1/2}I.

For t\geq1, both X_s+tI and Y_s+tI dominate c(s^2+t)I, with c>0 independent of s,t. The resolvent identity bounds their inverse difference by C(s^2+t)^{-2}, and therefore

\|P(t)\|_{\op}= \begin{cases} O(t^{-1/2}),&t\downarrow0,\\ O(t^{-3/2}),&t\to\infty. \end{cases} \tag{A.8}

These bounds prove the asserted convergence of N.

Fix t>0 and put \nabla=\partial_x-iB. We shall use the equation

(-\nabla^2+V+tI)\psi=0. \tag{A.9}

Matrix Riccati equations also appear in the commutation method for Schrödinger inequalities [2]. Here their role is to compute the integrated resolvent through boundary data.

For each v\in\C^n there is a unique H^1 solution of (A.9) on either half-line with \psi(0)=v. Indeed, the sesquilinear form

a_t(\phi,\psi)=\int \bigl(\langle\nabla\phi,\nabla\psi\rangle +\langle\phi,(V+tI)\psi\rangle\bigr)\,dx,

with inner products linear in the second variable, is coercive on H^1(\R;\C^n): its Fourier symbol X_s+tI dominates c_t(1+s^2)I. Zero extension gives coercivity on the trace-zero subspace of either half-line. Correcting any H^1 extension of v by the Riesz representation theorem gives the unique weak solution. The equation implies \psi''\in L^2, so this solution lies in H^2; both \psi and \psi' vanish at the infinite end.

Define the right and left boundary matrices S,T by

\nabla\psi(0+)=-Sv,\qquad \nabla\psi(0-)=Tv. \tag{A.10}

Integration by parts gives a_t(\psi_v,\psi_w)=\langle v,Sw\rangle on the right and a_t(\psi_v,\psi_w)=\langle v,Tw\rangle on the left. Thus S,T are Hermitian. Translation and uniqueness show that \nabla\psi=-S\psi throughout the right half-line and \nabla\psi=T\psi throughout the left half-line. Substituting these relations into (A.9), and allowing arbitrary boundary data, gives

V+tI=S^2+i[B,S]=T^2-i[B,T]. \tag{A.11}

Glue the two solutions with boundary value v at zero. The resulting continuous function has derivative jump -(S+T)v, and hence satisfies

(-\nabla^2+V+tI)\psi=\delta_0(S+T)v.

Fourier inversion, with forward kernel e^{-isx}, gives

v=\frac1{2\pi}\int_\R(X_s+tI)^{-1}\,ds\,(S+T)v =\tfrac12 R(t)(S+T)v.

The inverse symbol is O(s^{-2}), so its Fourier inverse is continuous and this evaluation at zero is justified. Therefore

L:=\tfrac12(S+T)=R^{-1}>0,\qquad Z:=\tfrac12(S-T)

satisfy (A.6), by adding and subtracting (A.11). The second equation in (A.6) determines Z uniquely from L, since L>0; in an eigenbasis of L, the map Z\mapsto LZ+ZL multiplies its (j,k) entry by the positive number L_{jj}+L_{kk}. This also proves the continuity of Z(t), because R(t), and hence L(t), is continuous.

The diagonal entries of that same equation give Z_{jj}=0 in an eigenbasis of L, so \tr Z=0. Multiplication on both sides by R=L^{-1} gives i[R,B]=-(ZR+RZ). Cyclicity of the trace now yields

\tr\bigl(R(V+tI)\bigr)=\tr L-\tr(RZ^2). \tag{A.12}

In particular, the correction \tr(RZ^2)=\tr(ZRZ) is nonnegative. We will also need the location of the spectrum of B+iS. The right solutions obey \psi'=i(B+iS)\psi. For an eigenvector with eigenvalue z, the solution is e^{izx}v; its square integrability forces \operatorname{Im}z>0.

A.2 A logarithmic integral

The next step converts the boundary matrices into a scalar identity that can be integrated in t. Define

F(t)=\frac{\tr V}{\sqrt t} -\frac1\pi\int_\R \log\frac{\det(X_s+tI)}{\det(Y_s+tI)}\,ds. \tag{A.13}

The determinants are positive, and the logarithmic ratio is O(|s|^{-2}) at infinity. Its derivative in t is the trace of the resolvent difference, with an integrable bound locally uniform for t>0. Thus the integral converges absolutely and F is continuously differentiable.

The first identity in (A.11) factors the symbol as

X_s+tI=(sI-B+iS)(sI-B-iS).

If u_j+iv_j are the eigenvalues of B+iS, counted with algebraic multiplicity, then v_j>0 and

\det(X_s+tI)=\prod_{j=1}^n\bigl((s-u_j)^2+v_j^2\bigr).

The denominator in (A.13) has the same form, with centers the eigenvalues of B and widths \sqrt t. Translations of the individual logarithms change their symmetric-cutoff integrals by o(1): for h(s)=\log(s^2+v^2),

\frac{d}{da}\int_{-M}^M h(s-a)\,ds =h(M+a)-h(M-a)\longrightarrow0

uniformly for bounded a. After centering the factors, the identity

\int_\R\log\frac{s^2+v^2}{s^2+w^2}\,ds=2\pi(v-w), \qquad v,w>0,

follows by differentiation in v and integration from w to v. Since \sum_jv_j=\tr S=\tr L, we obtain

F(t)=\frac{\tr V}{\sqrt t}-2\tr(L-\sqrt t I). \tag{A.14}

Set

G(t)=\tr(L-2\sqrt t I+tR). \tag{A.15}

Both functions are nonnegative. For G, apply \lambda-2\sqrt t+t/\lambda\geq0 to the positive eigenvalues \lambda of L. For F, take the trace of (A.6) and use (A.14) to obtain

F(t)=t^{-1/2}\tr\bigl((L-\sqrt t I)^2+Z^2\bigr)\geq0.

Equations (A.12) and (A.14) give the identity

\tr(PV)=F+G+\tr(RZ^2). \tag{A.16}

Every term on the right is nonnegative. The bounds (A.8) therefore show that F, G, and \tr(RZ^2) are integrable against t^\beta\,dt, and that t^{\beta+1}F(t) vanishes at both endpoints.

Differentiating (A.13) and using (A.14)–(A.15) gives

F'(t)=-\frac{\tr V}{2t^{3/2}}+\tr P(t), \qquad tF'(t)=-\tfrac12F(t)-G(t).

Integration by parts, with the endpoint limits just proved, yields \int_0^\infty t^\beta G\,dt =\sigma\int_0^\infty t^\beta F\,dt. Consequently, integration of (A.16) gives

\tr(NV)=q c_\sigma\int_0^\infty t^\beta G(t)\,dt +c_\sigma\int_0^\infty t^\beta\tr(RZ^2)\,dt. \tag{A.17}

It remains to express the first integral as \tr(N^q)/q plus a nonnegative remainder.

A.3 The noncommutative square

For a positive semidefinite matrix D, let

F_0(t,D)=\frac{\tr D}{\sqrt t} -2\tr\bigl((tI+D)^{1/2}-\sqrt t I\bigr).

For a scalar eigenvalue d\geq0, the corresponding summand is \int_0^d(t^{-1/2}-(t+y)^{-1/2})\,dy. Tonelli’s theorem and (A.2) therefore imply

c_\sigma\int_0^\infty t^\beta F_0(t,D)\,dt =\frac1p\tr(D^p). \tag{A.18}

Now expand the Hilbert–Schmidt square

\begin{align*} \mathcal D_D(t) &:=\bigl\|R^{-1/2}-R^{1/2}(tI+D)^{1/2}\bigr\|_{\HS}^2 \\ &=\tr\bigl(R^{-1}+R(tI+D)-2(tI+D)^{1/2}\bigr) \tag{A.19}\\ &=G(t)-\tr(P(t)D)+F_0(t,D).\end{align*}

No commutation is used: the cross terms cancel adjacent factors R^{-1/2}R^{1/2}, and cyclicity changes the remaining quadratic term into \tr(R(tI+D)). All three terms in the last line are integrable by (A.8), (A.16), and (A.18). Thus

c_\sigma\int_0^\infty t^\beta G(t)\,dt =\tr(ND)-\frac1p\tr(D^p) +c_\sigma\int_0^\infty t^\beta\mathcal D_D(t)\,dt. \tag{A.20}

When N\geq0, choose D=N^r. Since rp=q=1+r, the first two terms on the right equal \tr(N^q)/q. Substitution into (A.17) proves (A.7) and completes the proof of Theorem A.1.

If B and V commute, the symbol hypothesis implies V\geq bI. Simultaneous diagonalization then gives R(t)=(tI+V)^{-1/2}, N=V^\sigma, and Z=0. Both remainders vanish, as required by scalar equality.

B The regularized field and connecting paths

The finite-interval action argument requires a symmetric matrix path from K to -K whose derivative measures the difference between a matrix field and AA^{\mathsf T}. We construct both the field and the path here. These are the constructions of [11, Sections 4–5]; we include their proofs to make the analytic input to the equality argument self-contained. The positivity statement below also identifies the resolvent to which Theorem A.1 applies.

Throughout this appendix, K=\operatorname{diag}(k_1,\ldots,k_n) with k_i>0, \kappa=\max_i k_i, and \Sym_n denotes the real symmetric matrices. We use \beta=\sigma-\tfrac12 and the constant c_\sigma from (A.1).

B.1 A field with a scalar boundary integral

For \delta>0, define on y\geq0

f_\delta(y)=\frac{c_\sigma}{\pi}\int_0^\infty t^\beta \left(\frac1{t+\delta}-\frac1{t+\delta+y}\right)\,dt, \tag{B.1}

and extend to y<0 by the tangent line f_\delta'(0)y. The resulting function is C^1, strictly increasing, and concave. Indeed, for y\geq0,

f_\delta'(y)=a_\sigma(y+\delta)^{\beta-1}, \qquad a_\sigma=\frac{c_\sigma}{\pi} \int_0^\infty\frac{u^\beta}{(1+u)^2}\,du>0. \tag{B.2}

Both integrals converge since -\tfrac12<\beta<\tfrac12. The extension allows the functional calculus below even when its matrix argument has negative eigenvalues.

Set

\begin{split} Q_s(B)&=s^2I-2sB+K^2,\\ M_\delta(B)&=\lim_{R\to\infty}\int_{-R}^{R} \bigl(f_\delta(Q_s(B))-f_\delta(s^2)I\bigr)\,ds, \qquad B\in\Sym_n, \end{split} \tag{B.3}

where the symmetric cutoff cancels the leading term -2s f_\delta'(s^2)B, which is odd in s. The scalar counterpart is

\mu_\delta(z)=\int_\R \bigl(f_\delta(s^2+z)-f_\delta(s^2)\bigr)\,ds, \qquad z\in\R. \tag{B.4}

Proposition B.1 (Regularized field). The limit in (B.3) exists locally uniformly, and M_\delta:\Sym_n\to\Sym_n is locally Lipschitz. There is a C^1 function J_\delta:\Sym_n\to\R, normalized by J_\delta(0)=0, such that

dJ_\delta(B)[H]=-\tr(M_\delta(B)H). \tag{B.5}

The scalar function \mu_\delta is locally Lipschitz and strictly increasing, with \mu_\delta(0)=0, and

\mu_\delta(z)=(z+\delta)^\sigma-\delta^\sigma \qquad(z\geq0). \tag{B.6}

For every real unit vector e, and for every standard basis vector e_i, respectively,

\begin{align*} e^{\mathsf T}M_\delta(B)e &\leq\mu_\delta\bigl(e^{\mathsf T}K^2e -(e^{\mathsf T}Be)^2\bigr), \tag{B.7}\\ Be_i=ye_i\quad&\Longrightarrow\quad M_\delta(B)e_i=\mu_\delta(k_i^2-y^2)e_i. \tag{B.8}\end{align*}

For each diagonal sign matrix S,

M_\delta(SBS)=SM_\delta(B)S. \tag{B.9}

Finally,

\begin{split} J_\delta(-K)-J_\delta(K) &=\sum_{i=1}^n\int_{-k_i}^{k_i}\mu_\delta(k_i^2-s^2)\,ds\\ &\longrightarrow b_\sigma\sum_{i=1}^n k_i^{2\sigma+1} \qquad(\delta\downarrow0). \end{split} \tag{B.10}

Proof. We first justify the matrix integral, including its local Lipschitz dependence. If a scalar function h is Lipschitz on an interval containing the spectra of Hermitian matrices X,Y, then

\|h(X)-h(Y)\|_{\HS}\leq\operatorname{Lip}(h)\|X-Y\|_{\HS}. \tag{B.11}

To see this, use eigenbases e_i of X and v_j of Y. The mixed matrix entries of the two differences are (h(\lambda_i)-h(\nu_j))\langle e_i,v_j\rangle and (\lambda_i-\nu_j)\langle e_i,v_j\rangle; square the scalar Lipschitz inequality and sum over i,j.

On a bounded set of B’s the spectrum of E_s(B)=-2sB+K^2 is contained in [-a|s|,a|s|] for all sufficiently large |s|. For

h_s(y)=f_\delta(s^2+y)-f_\delta(s^2)-f_\delta'(s^2)y,

Equation (B.2) gives \sup_{|y|\leq a|s|}|h_s'(y)|=O(|s|^{2\beta-3}). It follows from (B.11) that

f_\delta(Q_s(B))-f_\delta(s^2)I =-2s f_\delta'(s^2)B+T_s(B),

where both \|T_s(B)\|_{\HS} and the local Lipschitz constant of T_s are O(|s|^{2\beta-2}). For the first bound, include f_\delta'(s^2)K^2 in T_s; for the second, apply (B.11) to h_s(E_s(B)) and use E_s(B_1)-E_s(B_2)=-2s(B_1-B_2). Because 2\beta-2<-1, these remainders are integrable at infinity. The odd term cancels at each symmetric cutoff. On bounded s-intervals, (B.11) applies directly to f_\delta. This proves the asserted convergence and regularity.

For the primitive, choose a scalar antiderivative g_\delta'=f_\delta. Trace differentiation gives d\tr(g_\delta(X))[H]=\tr(f_\delta(X)H). This formula follows for polynomials by cyclicity and for g_\delta by approximation in C^1 on compact spectral intervals. For s\ne0, the function

B\longmapsto \frac{\tr(g_\delta(Q_s(B))-g_\delta(K^2))}{2s} +f_\delta(s^2)\tr B

has differential -\tr((f_\delta(Q_s(B))-f_\delta(s^2)I)H). At s=0 that differential is constant in B and also has a primitive. Thus the negative of every finite-cutoff field has zero integral around each closed piecewise smooth curve in \Sym_n. Local uniform convergence passes this property to -M_\delta. Path integration, starting at zero, defines J_\delta and proves (B.5).

For bounded z, the integrand in (B.4) and its Lipschitz constant in z are O(|s|^{2\beta-2}) at infinity. This proves absolute convergence and local Lipschitz continuity of \mu_\delta. Strict increase and \mu_\delta(0)=0 follow from the same properties of f_\delta. For z\geq0, Tonelli’s theorem applied to (B.1) gives

\mu_\delta(z)=c_\sigma\int_0^\infty t^\beta \bigl((t+\delta)^{-1/2}-(t+\delta+z)^{-1/2}\bigr)\,dt.

The normalization (A.1), after scaling, evaluates this as (B.6).

Translations in the variable s remain legitimate with a symmetric cutoff. More precisely, for fixed a,z\in\R,

\lim_{R\to\infty}\int_{-R}^{R} \bigl(f_\delta((s-a)^2+z)-f_\delta(s^2)\bigr)\,ds =\mu_\delta(z). \tag{B.12}

Indeed F_z(s)=f_\delta(s^2+z) is even and F_z'(s)=O(|s|^{2\beta-1})\to0 at infinity. Pairing the two short intervals produced by a translation bounds the difference between the shifted and unshifted cutoff integrals by

|a|^2\sup_{R-|a|\leq u\leq R+|a|}|F_z'(u)|,

which tends to zero.

Scalar concavity in an eigenbasis of Q_s(B) now gives

e^{\mathsf T}f_\delta(Q_s(B))e \leq f_\delta(e^{\mathsf T}Q_s(B)e).

The scalar argument on the right is (s-e^{\mathsf T}Be)^2+e^{\mathsf T}K^2e-(e^{\mathsf T}Be)^2. Integration and (B.12) prove (B.7). If Be_i=ye_i, functional calculus gives equality in the corresponding coordinate, proving (B.8). Since SK^2S=K^2, conjugation inside the defining integral proves (B.9).

On diagonal matrices, (B.5) and (B.8) read

dJ_\delta(\operatorname{diag}(b_1,\ldots,b_n)) =-\sum_i\mu_\delta(k_i^2-b_i^2)\,db_i.

Integrating from K to -K gives the first equality in (B.10). For z\geq0, 0\leq\mu_\delta(z)\leq z^\sigma and \mu_\delta(z)\to z^\sigma. Dominated convergence and the substitution s=k_i u give its stated limit.

The field is defined on all symmetric matrices, but the action argument compares it with a positive matrix AA^{\mathsf T}. At such values its directional bound forces positivity of the entire quadratic symbol Q_s(B). This is the condition needed for the trace deficit formula.

Proposition B.2 (Positive values of the field). If M=M_\delta(B)\geq0, then

Q_s(B)\geq0\quad(s\in\R),\qquad 0\leq M\leq\kappa^{2\sigma}I. \tag{B.13}

Set V=K^2-B^2+\delta I and use B,V in (A.4) and (A.5). Then the symbol (sI-B)^2+V=Q_s(B)+\delta I is bounded below by \delta I, and

N=M+\delta^\sigma I. \tag{B.14}

In particular, the hypotheses of Theorem A.1 hold.

Proof. By (B.7), positivity of M and strict increase of \mu_\delta imply e^{\mathsf T}K^2e\geq(e^{\mathsf T}Be)^2 for every real unit vector e. Completing the scalar square gives

e^{\mathsf T}Q_s(B)e=(s-e^{\mathsf T}Be)^2 +e^{\mathsf T}K^2e-(e^{\mathsf T}Be)^2\geq0.

Thus Q_s(B)\geq0, also as a Hermitian matrix on \C^n. Moreover, (B.7) gives M\leq\mu_\delta(\kappa^2)I\leq\kappa^{2\sigma}I, using (a+b)^\sigma\leq a^\sigma+b^\sigma.

Write Y_s=(sI-B)^2. Diagonalization of B and (B.12) allow replacement of the scalar subtraction f_\delta(s^2)I in (B.3) by f_\delta(Y_s). Since both Q_s(B) and Y_s are positive, their difference under f_\delta is, by (B.1),

\frac{c_\sigma}{\pi}\int_0^\infty t^\beta \left((Y_s+(t+\delta)I)^{-1} -(Q_s(B)+(t+\delta)I)^{-1}\right)\,dt.

For fixed B,\delta, both matrices being inverted are bounded below by c(1+t+s^2)I. Their difference is K^2-B^2, so the resolvent identity bounds the norm of the integrand by C t^\beta(1+t+s^2)^{-2}. Integrating first in s yields C't^\beta(1+t)^{-3/2}, which is integrable on (0,\infty). Fubini’s theorem is therefore applicable and gives

M=c_\sigma\int_0^\infty t^\beta \bigl((t+\delta)^{-1/2}I-R(t)\bigr)\,dt.

Subtracting this expression from (A.5) and scaling (A.1) gives (B.14).

B.2 Choosing the lower triangular coefficient matrix

Let \mathcal L_n be the real lower triangular n\times n matrices. Their dimension equals that of \Sym_n. This dimension match allows us to prescribe a symmetric terminal value by choosing C\in\mathcal L_n. At a simple initial problem there is one choice up to signs of the rows. Continuation preserves the parity of this number, and hence produces the required terminal value.

Proposition B.3 (Connecting path). Let \Omega=(x_-,x_+) be bounded and let U\in H^1_0(\Omega;\R^{n\times d}), where n,d\geq1, satisfy

\int_\Omega UU^{\mathsf T}\,dx=I_n.

For every \delta,\varepsilon>0 there are C_\varepsilon\in\mathcal L_n and B_\varepsilon\in C^1(\overline\Omega;\Sym_n) such that, with A_\varepsilon=C_\varepsilon U,

\varepsilon B_\varepsilon' =M_\delta(B_\varepsilon)-A_\varepsilon A_\varepsilon^{\mathsf T}, \qquad B_\varepsilon(x_-)=K,\quad B_\varepsilon(x_+)=-K. \tag{B.15}

They satisfy

\sup_{x\in\overline\Omega}\|B_\varepsilon(x)\|_{\op}\leq\kappa, \qquad \sup_{0<\varepsilon\leq1}\|C_\varepsilon\|_{\HS}<\infty, \tag{B.16}

where the second bound is for fixed \delta,K,\Omega.

Proof. Use the continuous representative of U. Choose a smooth, nonnegative, compactly supported cutoff \chi on \Sym_n, equal to one on \{B:\|B\|_{\op}\leq\kappa\} and invariant under conjugation by diagonal sign matrices. Averaging a cutoff over the finite sign group produces such a function. The truncated field \widehat M=\chi M_\delta is bounded and globally Lipschitz.

Fix \varepsilon>0. For C\in\mathcal L_n and \theta\in[0,1], the equation

\varepsilon B'=\theta\widehat M(B)-(CU)(CU)^{\mathsf T}, \qquad B(x_-)=K \tag{B.17}

has a unique C^1 solution on \overline\Omega. Define the continuous endpoint map

\Phi(C,\theta)=B(x_+)+K\in\Sym_n.

Let \mathcal G be the group of diagonal sign matrices, acting by C\mapsto SC on \mathcal L_n and by conjugation on \Sym_n. Equivariance of the field and uniqueness of the ODE give

\Phi(SC,\theta)=S\Phi(C,\theta)S. \tag{B.18}

We record the three facts needed for continuation: compactness of the zero set, freeness of the sign action there, and one regular orbit of zeros at \theta=0. At a zero, integration of (B.17) gives

CC^{\mathsf T}=2\varepsilon K +\theta\int_\Omega\widehat M(B(x))\,dx. \tag{B.19}

Consequently all zeros lie in a bounded set, and their joint set in \mathcal L_n\times[0,1] is compact. For 0<\varepsilon\leq1, this calculation gives the uniform bound

\|C\|_{\HS}^2\leq2\tr K +n|\Omega|\sup_{B\in\Sym_n}\|\widehat M(B)\|_{\op}. \tag{B.20}

No row of C can vanish at a zero. Otherwise the reflection changing only row i would fix C; ODE uniqueness and (B.18) would force Be_i=y e_i throughout the interval. Equation (B.8) would then give

\varepsilon y'=\theta\chi(B(x))\mu_\delta(k_i^2-y^2), \qquad y(x_-)=k_i.

The coefficient \chi(B(x)) is continuous and the right side is locally Lipschitz in y. Uniqueness forces y\equiv k_i, contradicting y(x_+)=-k_i. Thus the action of \mathcal G on the zero set is free.

At \theta=0 one has

\Phi(C,0)=2K-\varepsilon^{-1}CC^{\mathsf T}. \tag{B.21}

Its lower triangular zeros are exactly C=\operatorname{diag}(d_1,\ldots,d_n) with d_i=\pm\sqrt{2\varepsilon k_i}. Indeed, the first row of CC^{\mathsf T}=2\varepsilon K fixes |d_1| and forces all other entries of the first column to vanish, and induction does the same for subsequent columns. These 2^n zeros form one sign orbit. At each, the derivative in a lower triangular direction H has diagonal entries -2\varepsilon^{-1}d_i H_{ii} and lower off-diagonal entries -\varepsilon^{-1}d_j H_{ij} for i>j. It is therefore an isomorphism \mathcal L_n\to\Sym_n.

We next justify the continuation using only smooth approximation and the regular-value argument for parity [10, Sections 2–4]. Suppose there were no zero at \theta=1. Compactness and freeness give a bounded invariant open set O\subset\mathcal L_n containing the projection of every zero, whose closure lies where all rows are nonzero. There is a positive lower bound for \|\Phi\|_{\HS} on

(\partial O\times[0,1])\ \cup\ (\overline O\times\{1\}). \tag{B.22}

Reparametrize \theta by a smooth map equal to zero near zero and equal to one at one. The resulting map F agrees with (B.21) on an initial collar and retains the gap on (B.22).

Extend F constantly beyond the two ends of the parameter interval, smooth by convolution, and splice to (B.21) in a smaller initial collar. Averaging the approximation \Psi_0 in the form

\Psi(C,\theta)=\frac1{|\mathcal G|} \sum_{S\in\mathcal G}S\Psi_0(SC,\theta)S

gives a smooth equivariant approximation \Psi that still equals the initial map on that collar. It can be made uniformly close enough on \overline O\times[0,1] to preserve the positive gap.

Freeness permits an equivariant perturbation with arbitrary target directions. At each C_0\in\overline O, choose a ball whose distinct sign translates are disjoint, and a smooth bump b supported in this ball with b(C_0)=1. For H\in\Sym_n the map

V_H(C)=\sum_{S\in\mathcal G}b(SC)SHS

is equivariant and satisfies V_H(C_0)=H. Choose a basis of target matrices and then a finite collection of such neighborhoods covering \overline O. This gives finitely many smooth equivariant maps V_1,\ldots,V_N whose values span \Sym_n at every point of \overline O.

Let h\geq0 be smooth, vanish near zero, and be positive outside the collar where \Psi is the initial map. Choose it so that every zero of h lies within that collar, and set

\Psi_\alpha(C,\theta) =\Psi(C,\theta)+h(\theta)\sum_{j=1}^{N}\alpha_jV_j(C).

For \alpha in a sufficiently small open ball, the gap on (B.22) persists. At a zero of this family with 0<\theta<1, its full differential in (C,\theta,\alpha) is onto: when h(\theta)>0 the parameter directions span the target, and when h(\theta)=0 the derivative in C is the isomorphism computed for (B.21). Its interior zero set is consequently a smooth manifold. Sard’s theorem [13], applied to projection of this manifold onto the parameter ball, gives arbitrarily small \alpha for which zero is a regular value of (C,\theta)\mapsto\Psi_\alpha(C,\theta). For completeness, if the full derivative is (L_1,L_2) in the (C,\theta) and \alpha directions, regularity of that projection means that each w admits v with L_1v+L_2w=0. Hence \operatorname{ran}L_2\subset \operatorname{ran}L_1, and surjectivity of (L_1,L_2) implies surjectivity of L_1.

For such an \alpha, the zero set in O\times[0,1] is a compact smooth one-dimensional manifold with boundary. The gap excludes boundary zeros except at \theta=0, where the initial collar gives exactly the 2^n regular zeros above. The free sign action has a quotient that is again a compact one-dimensional manifold with boundary: a neighborhood disjoint from its nontrivial translates supplies the local interval or half-interval chart. All 2^n boundary points form one orbit, so the quotient has exactly one boundary point. This is impossible, since a compact one-dimensional manifold is a finite union of circles and closed intervals. Therefore the original map \Phi(\cdot,1) has a zero.

It remains to remove the cutoff. For the path at this zero and any fixed real unit vector e, put y=e^{\mathsf T}Be. Whenever |y|>\kappa, Equation (B.7) yields

e^{\mathsf T}M_\delta(B)e \leq\mu_\delta(e^{\mathsf T}K^2e-y^2)<0.

Since \chi\geq0 and (CU)(CU)^{\mathsf T}\geq0, the ODE implies y'\leq0 there. Both endpoint values lie in [-\kappa,\kappa]. An excursion above \kappa cannot start from \kappa while y is nonincreasing; an excursion below -\kappa cannot return to -\kappa while y is nonincreasing. The two endpoint conditions therefore rule out both excursions. This holds for every e, so \|B(x)\|_{\op}\leq\kappa. Consequently \chi(B)=1, giving (B.15), and (B.20) supplies the remaining assertion in (B.16).

References

  1. [1]Michael Aizenman and Elliott H. Lieb, On semi-classical bounds for eigenvalues of Schrödinger operators, Physics Letters A 66 (1978), no. 6, 427–429. doi:10.1016/0375-9601(78)90385-7.
  2. [2]Rafael Benguria and Michael Loss, A simple proof of a theorem of Laptev and Weidl, Mathematical Research Letters 7 (2000), no. 2–3, 195–203. doi:10.4310/MRL.2000.v7.n2.a5.
  3. [3]Rupert L. Frank, David Gontier and Mathieu Lewin, Optimizers for the finite-rank Lieb–Thirring inequality, American Journal of Mathematics 147 (2025), no. 2, 503–560. doi:10.1353/ajm.2025.a954649.
  4. [4]Dirk Hundertmark, Ari Laptev and Timo Weidl, New bounds on the Lieb–Thirring constants, Inventiones Mathematicae 140 (2000), no. 3, 693–704. doi:10.1007/s002220000077.
  5. [5]Dirk Hundertmark, Elliott H. Lieb and Lawrence E. Thomas, A sharp bound for an eigenvalue moment of the one-dimensional Schrödinger operator, Advances in Theoretical and Mathematical Physics 2 (1998), no. 4, 719–731. doi:10.4310/ATMP.1998.v2.n4.a2.
  6. [6]Joseph B. Keller, Lower bounds and isoperimetric inequalities for eigenvalues of the Schrödinger equation, Journal of Mathematical Physics 2 (1961), no. 2, 262–266. doi:10.1063/1.1703708.
  7. [7]Ari Laptev and Timo Weidl, Sharp Lieb–Thirring inequalities in high dimensions, Acta Mathematica 184 (2000), no. 1, 87–111. doi:10.1007/BF02392782.
  8. [8]Elliott H. Lieb and Walter E. Thirring, Bound for the kinetic energy of fermions which proves the stability of matter, Physical Review Letters 35 (1975), no. 11, 687–689; erratum, 35 (1975), 1116. doi:10.1103/PhysRevLett.35.687.
  9. [9]Elliott H. Lieb and Walter E. Thirring, Inequalities for the moments of the eigenvalues of the Schrödinger Hamiltonian and their relation to Sobolev inequalities, in Studies in Mathematical Physics: Essays in Honor of Valentine Bargmann, Elliott H. Lieb, Barry Simon and Arthur S. Wightman (eds.), Princeton University Press, Princeton, NJ, 1976, 269–303.
  10. [10]John W. Milnor, Topology from the Differentiable Viewpoint, University Press of Virginia, Charlottesville, VA, 1965.
  11. [11]OpenAI, Sharp one-dimensional Lieb–Thirring inequalities for matrix potentials, OpenAI Math Release preprint PDF, 2026. Reading view on this site: Sharp one-dimensional Lieb–Thirring inequalities for matrix potentials.
  12. [12]Larry Read and Marvin R. Schulz, The sharp one-dimensional Lieb–Thirring inequality for the sum of eigenvalues, arXiv:2609.10478v2, September 14, 2026.
  13. [13]Arthur Sard, The measure of the critical values of differentiable maps, Bulletin of the American Mathematical Society 48 (1942), 883–890. doi:10.1090/S0002-9904-1942-07811-6.