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Triple Products of Eigenfunctions and Schrodinger/Witten Operators

[VERIFIED] Last updated by Joe Schaefer on Fri, 28 Aug 2026    source
 

Dynamics

Author

Joe Schaefer

Dedication

To Autumn

Abstract

Using elementary techniques from Geometric Analysis, Partial Differential Equations, and Abelian CC^*Algebras, we uncover a novel, yet familiar, global geometric discriminant – namely the indexed set of integrals of triple products of eigenfunctions of the Schrodinger/Witten Operator, to precisely characterize which isospectral Schrodinger/Witten Operators are isometric.

Introduction

Let (M,g)(M,g) be a smooth, connected, complete Riemannian manifold (possibly non-compact, possibly of infinite volume). Fix a real potential VC(M)V\in C^\infty(M) which is bounded below and proper in the sense

V(x)+as xV(x)\to +\infty\qquad\text{as }x\to\infty

(i.e., x:V(x)C{x:V(x)\le C} is compact for every CC). Let

H=Δg+VH=-\Delta_g+V

be the associated Schrodinger operator, essentially self-adjoint on Cc(M)C_c^\infty(M). Under these hypotheses it is classical that σ(H)=σdisc(H)=λ0<λ1λ2+\sigma(H)=\sigma_{\mathrm{disc}}(H)={\lambda_0\lt\lambda_1\le\lambda_2\le\cdots}\to+\infty, each eigenvalue of finite multiplicity; there is an orthonormal basis eii=0L2(M,dvolg){e^i}_{i=0}^\infty\subset L^2(M,d\mathrm{vol}_g) of smooth eigenfunctions,

Hei=λiei.He^i=\lambda_i e^i.

(The same conclusions hold for Δg-\Delta_g itself on some complete manifolds of finite volume with no continuous spectrum, but the confining potential makes the analysis cleaner.)
Define the triple products exactly as in the compact case:

Mi,j,k:=eiej,ekL2=Meiej ek dvolg.M^{i,j,k}:=\langle e^i e^j,e^k\rangle_{L^2}=\int_M e^i e^j\ \overline{e^k}\ d\mathrm{vol}_g.

Because the eigenfunctions are Schwartz-class at infinity in the sense that they decay faster than any polynomial in VV (Agmon estimates [Agmon1982]/ weighted Sobolev [TaylorPDE1]), the products eieje^i e^j lie in L2L^2 and the integrals converge absolutely.

Results

Theorem

Let (M,g,V)(M,g,V) and (N,h,W)(N,h,W) be two such data, with isospectral Schrödinger operators HMH_M and HNH_N. Suppose there exist orthonormal eigenbases ei{e^i} of HMH_M and fi{f^i} of HNH_N, ordered by non-decreasing eigenvalues, such that

MMi,j,k=MNi,j,ki,j,k.M_M^{i,j,k}=M_N^{i,j,k}\qquad\forall\qquad i,j,k.

Then there is a diffeomorphism F:NMF:N\to M with Fg=hF^*g=h and VF=WV\circ F=W.

Corollary

Let (M,g)(M,g) be a complete connected Riemannian manifold and φC(M)\varphi\in C^\infty(M) a weight such that the Witten operator

Lφu=Δgu+φ,uL_\varphi u=-\Delta_g u+\langle\nabla\varphi,\nabla u\rangle

is essentially self-adjoint and bounded below on Cc(M)C_c^\infty(M), with

σ(Lφ)=σdisc(Lφ)=ν0=0<ν1ν2+\sigma(L_\varphi)=\sigma_{\mathrm{disc}}(L_\varphi)={\nu_0=0<\nu_1\le\nu_2\le\cdots}\to+\infty

in L2(M,eφ dvolg)L^2(M,e^{-\varphi}\ d\mathrm{vol}_g). (This holds whenever φ\varphi is confining in the Bakry–Émery sense: e.g. Ricg+HessφK\operatorname{Ric}_g+\operatorname{Hess}\varphi\ge K and φ(x)+\varphi(x)\to+\infty as xx\to\infty.) Let {fi}i=0\set{f^i} _{i=0}^\infty be an orthonormal eigenbasis,

Lφfi=νifi,Mfifj eφ dvolg=δij,L_\varphi f^i=\nu_i f^i,\qquad\int_M f^i\overline{f^j}\ e^{-\varphi}\ d\mathrm{vol}_g=\delta^{ij},

ordered by nondecreasing eigenvalues, and set

Wi,j,k:=Mfifjfk eφ dvolg=fifj,fkL2(eφvol).W^{i,j,k}:=\int_M f^i f^j\overline{f^k}\ e^{-\varphi}\ d\mathrm{vol}g=\langle f^if^j,f^k\rangle{L^2(e^{-\varphi}\mathrm{vol})}.

Let (N,h,ψ)(N,h,\psi) be a second such triple, with Witten operator LψL_\psi isospectral to LφL_\varphi, and suppose there is an eigenbasis ui{u^i} of LψL_\psi with the same eigenvalues and

Nuiujuk eψ dvolh=Wi,j,kfor all i,j,k.\int_N u^i u^j\overline{u^k}\ e^{-\psi}\ d\mathrm{vol}_h=W^{i,j,k}\quad\text{for all }i,j,k.

Then there exists a diffeomorphism F:NMF:N\to M such that
Fg=h,ψ=φF+logμ(M)μ(N).F^*g=h,\qquad \psi=\varphi\circ F+\log \frac{\mu(M)}{\mu(N)}.
In particular the weighted Riemannian manifolds (M,g,eφvolg)(M,g,e^{-\varphi}\mathrm{vol}_g) and (N,h,eψvolh)(N,h,e^{-\psi}\mathrm{vol}_h) are isometric.

Remark

The Witten Laplacian on pp-forms is the Hodge Laplacian of the weighted manifold plus

tHessφ#p+t2φ2.t\operatorname{Hess}\varphi\#_p+t^2\lvert\nabla\varphi\rvert^2.

Once (M,g,φ)(M,g,\varphi) is reconstructed from the scalar array Wi,j,kW^{i,j,k}, the operators Lφ(p)L_{\varphi}^{(p)} are determined, so their spectra and eigenform pairings against scalar eigenfunctions are invariants, not additional moduli.

Preliminaries

Let A0L2(M)\mathcal{A}_0\subset L^2(M) be the algebraic span of the eigenfunctions. Finite linear combinations

ϕ=i=0Nϕ^(i) ei\phi=\sum_{i=0}^N\hat\phi(i)\ e^i

are dense in L2L^2 and, by elliptic regularity plus the decay of eigenfunctions, lie in CC0(M)C^\infty\cap C_0(M). Pointwise multiplication is

ϕψ=k(i,jϕ^(i)ψ^(j)Mi,j,k)ek.\phi\psi=\sum_k\Bigl(\sum_{i,j}\hat\phi(i)\hat\psi(j)M^{i,j,k}\Bigr)e^k.

Thus the structure constants determine the product of any two finite eigenfunction expansions. The same identity holds on NN. Consequently the linear map

F:A0(M)A0(N),eifi\vec F:\mathcal{A}_0(M)\to\mathcal{A}_0(N),\qquad e^i\mapsto f^i

is a unital algebra homomorphism for pointwise multiplication (the constant function is a multiple of the ground state only if VV is constant; in general F\vec F need not send 11 to 11, but it preserves the product of any two functions that can be so expanded). Characteristic functions of sublevel sets of VV can be approximated in L2L^2 by functional calculus of HH, so F\vec F also preserves characteristic functions of sets of finite measure in the L2L^2 sense.

This is identical to the compact calculation; the only extra ingredient is that the eigenfunction expansion of a compactly supported smooth function still converges rapidly enough for the triple-product formula to be justified (which follows from the same elliptic estimates that give λiNei0\lambda_i^{N}|e^i|_\infty\to 0 locally, plus Agmon decay at infinity).

Proof of Theorem

(Following [JS24]) For sufficiency, we now consider the linear, bijective orthonormal eigenfunction basis map F\vec{F} from C(M)C^\infty(M) to C(N)C^\infty(N) and note that from the calculations in Preliminaries section above, F\vec{F} preserves pointwise products for smooth functions (and preserves characteristic functions when extended to L2(M,g)L^2(M,g)) by the premise that {Mi,j,k}\set{M^{i,j,k}} is invariant under this map.

Lemma

F\vec F preserves the uniform norm on the span of the eigenfunctions, hence extends to an isometric *-homomorphism

F:C0(M)A0C0(N).\vec F:C_0(M)\supset\overline{\mathcal{A}_0}^{|\cdot|_\infty}\longrightarrow C_0(N).

Proof of Lemma

On a compact manifold one uses a smooth partition of unity and the fact that a=1|a|_\infty=1 for a partition function $a$ is detected by ap=1|a^p|_\infty=1 for all pp, which is visible in the Fourier coefficients because the limiting characteristic function of a=1{a=1} has L2L^2-mass.

In the non-compact setting replace a global partition of unity by a sequence of cutoffs χR\chi_R that equal 11 on VR{V\le R} and vanish outside VR+1{V\le R+1}. On each such “almost-compact” region the same argument applies: if ϕ=c|\phi|_\infty=c is attained on a set of positive measure inside VR{V\le R}, the powers

ϕp/ϕp\phi^p/|\phi|_\infty^p

converge in Lloc2L^2_{\mathrm{loc}} to a characteristic function, and F\vec F preserves that limit because it preserves all triple products. Sending RR\to\infty and using that every function in C0(M)C_0(M) is uniformly small outside a large sublevel set of VV gives F(ϕ)=ϕ|\vec F(\phi)|_\infty=|\phi|_\infty.

Now we apply the Gelfand-Naimark-Segal Representation Theorem (in contravariant functor form) for Abelian CC^* algebras C0(N),C0(M)C_0(N), C_0(M) [JC19] to represent this isomorphism F\vec{F} by a homeomorphism FF between NN and MM. Since F\vec{F} is bijective on smooth functions, FF too must be smooth.

As this now diffeomorphism preserves eigenvalues and eigenfunctions (by hypothesis on F(f)=fF\vec{F}(f) = f \circ F), it must preserve the Schrodinger operator on smooth functions. By construction

F(ϕ)=ϕF\vec F(\phi)=\phi\circ F

on the eigenbasis, hence on all finite combinations. Therefore

HN(ϕF)=(HMϕ)FH_N(\phi\circ F)=(H_M\phi)\circ F

for every eigenfunction ϕ\phi, and by density for every Schwartz-class function. In particular FF pulls eigenfunctions of HMH_M back to eigenfunctions of HNH_N with the same eigenvalues.

Writing H=Δ+VH=-\Delta+V in local coordinates, the principal symbol of HH is the same as that of Δ-\Delta, namely the cometric gijξiξjg^{ij}\xi_i\xi_j. An elliptic operator that is intertwined by a diffeomorphism has its principal symbol pulled back. Hence

Fg=h.F^*g=h.

The zeroth-order terms then give VF=WV\circ F=W.

This completes the proof of the Theorem. As the proof of the Corollary is redundant, it is omitted.

Example

On M=RM=\mathbb{R} with the Euclidean metric, take

H=d2dx2+x2.H=-\frac{d^2}{dx^2}+x^2.

The potential V(x)=x2V(x)=x^2 is smooth, bounded below, and V(x)+V(x)\to+\infty as x|x|\to\infty. Hence σess(H)=\sigma_{\mathrm{ess}}(H)=\emptyset. The spectrum is

λn=2n+1,n=0,1,2,\lambda_n=2n+1,\qquad n=0,1,2,\dots

(each of multiplicity one). The corresponding L2(R)L^2(\mathbb{R})-normalized eigenfunctions are the Hermite functions

ψn(x)=(2nn! π)1/2Hn(x) ex2/2,\psi_n(x)=\bigl(2^n n!\ \sqrt{\pi}\bigr)^{-1/2}H_n(x)\ e^{-x^2/2},

where HnH_n are the physicist’s Hermite polynomials. They form an orthonormal basis of L2(R)L^2(\mathbb{R}), lie in the Schwartz class S(R)C0(R)\mathcal{S}(\mathbb{R})\subset C_0(\mathbb{R}), and satisfy the Agmon decay that makes every pointwise product ψiψj\psi_i\psi_j square-integrable.

Triple Products

Because the eigenfunctions are real,

Mi,j,k=ψiψj,ψk=ψi(x)ψj(x)ψk(x) dx.M^{i,j,k}=\langle\psi_i\psi_j,\psi_k\rangle=\int_{-\infty}^{\infty}\psi_i(x)\psi_j(x)\psi_k(x)\ dx.

These integrals vanish unless i+j+ki+j+k is even (parity) and the three indices satisfy a triangle-type constraint coming from the linearization of Hermite polynomials. The linearization formula

Hn(x)Hm(x)=r=0min(n,m)(nr)(mr)r! 2r Hn+m2r(x)H_n(x)H_m(x)=\sum_{r=0}^{\min(n,m)}\binom{n}{r}\binom{m}{r}r!\ 2^r\ H_{n+m-2r}(x)

together with the Gaussian weight converts, after normalizing, into an explicit formula for Mi,j,kM^{i,j,k}. Equivalently, the generating-function identity

ex2Ha(x)Hb(x)Hc(x) dx=π 2Na! b! c!(Na)!(Nb)!(Nc)!\int_{-\infty}^{\infty}e^{-x^2}H_a(x)H_b(x)H_c(x)\ dx=\sqrt{\pi}\ 2^N\frac{a!\ b!\ c!}{(N-a)!(N-b)!(N-c)!}

(when a+b+c=2Na+b+c=2N is even and each factorial in the denominator is defined and non-negative, and 00 otherwise) yields Mi,j,kM^{i,j,k} after inserting the normalization constants of the ψn\psi_n. In particular:

Mn,n,0=ψn2ψ0 dx>0M^{n,n,0}=\int\psi_n^2\psi_0\ dx>0 (the ground state ψ0=π1/4ex2/2\psi_0=\pi^{-1/4}e^{-x^2/2} is a strictly positive Gaussian);
the map ψiψj=kMi,j,kψk\psi_i\psi_j=\sum_k M^{i,j,k}\psi_k is the exact multiplication rule in the Hermite basis.

So the structure constants of pointwise multiplication on the dense subspace span ψnC0(R)\mathrm{span}\ {\psi_n}\subset C_0(\mathbb{R}) are known in closed form.

What the theorem says

Suppose (R,g,W)(\mathbb{R},g,W) is another complete Riemannian line (so g=e2ϕ(x) dx2g=e^{2\phi(x)}\ dx^2 in some coordinate) with a smooth confining potential WW, and suppose its Schrödinger operator Δg+W-\Delta_g+W is isospectral to HH and admits an eigenbasis fn{f_n} with the same triple products fifj,fk=Mi,j,k.\langle f_i f_j,f_k\rangle=M^{i,j,k}.

The discrete-spectrum argument then produces a diffeomorphism F:RRF:\mathbb{R}\to\mathbb{R} such that

Fg=dx2,WF=x2.F^*g=dx^2,\qquad W\circ F=x^2.

In one dimension this is almost tautological once the algebra is identified, but the mechanism is visible by hand:

Finite Hermite combinations are dense in C0(R)C_0(\mathbb{R}) for the uniform norm (Stone–Weierstrass on each compact plus Gaussian decay at infinity). The numbers Mi,j,kM^{i,j,k} determine the product of any two such combinations, hence determine a CC^*-isomorphism

C0(R)C0(R),ψnfn.C_0(\mathbb{R})\longrightarrow C_0(\mathbb{R}),\qquad \psi_n\mapsto f_n.

Gelfand–Naimark supplies a homeomorphism of the underlying locally compact spaces; smoothness of the eigenfunctions upgrades it to a diffeomorphism FF. Intertwining of HH forces the principal symbol (the cometric) and the zeroth-order term (the potential) to match.

Because every eigenspace is one-dimensional, the singular-value packaging collapses to the absolute values Mi,j,k|M^{i,j,k}| together with a consistent choice of signs (the “diagonal litmus” of the compact paper: the products Mi,i,kM^{i,i,k} determine the even part of the algebra and fix most signs).

Explicit Formula

Mi,j,k=ψiψj,ψk=Rψi(x)ψj(x)ψk(x) dx=NiNjNkRHi(x)Hj(x)Hk(x) e3x2/2 dx,M^{i,j,k}=\langle\psi_i\psi_j,\psi_k\rangle=\int_{\mathbb{R}}\psi_i(x)\psi_j(x)\psi_k(x)\ dx=N_i N_j N_k\int_{\mathbb{R}}H_i(x)H_j(x)H_k(x)\ e^{-3x^2/2}\ dx,

where Nn=(2nn!π)1/2N_n=(2^n n!\sqrt{\pi})^{-1/2}.

Mi,j,k=0M^{i,j,k}=0 unless both of the following hold – parity: i+j+ki+j+k is even; triangle: ijki+j|i-j|\le k\le i+j (and cyclic permutations).

These are the oscillator analogues of the Clebsch–Gordan support conditions.

Change variables x=2/3 yx=\sqrt{2/3}\ y. Then

RHi(x)Hj(x)Hk(x) e3x2/2 dx=23RHi(23 y)Hj(23 y)Hk(23 y) ey2 dy.\int_{\mathbb{R}}H_i(x)H_j(x)H_k(x)\ e^{-3x^2/2}\ dx=\sqrt{\frac{2}{3}}\int_{\mathbb{R}}H_i\Bigl(\sqrt{\tfrac{2}{3}}\ y\Bigr)H_j\Bigl(\sqrt{\tfrac{2}{3}}\ y\Bigr)H_k\Bigl(\sqrt{\tfrac{2}{3}}\ y\Bigr)\ e^{-y^2}\ dy.

Each scaled polynomial expands by the finite identity

Hn(γy)==0n/2γn2(γ21)(n2)(2)!! Hn2(y),H_n(\gamma y)=\sum_{\ell=0}^{\lfloor n/2\rfloor}\gamma^{n-2\ell}(\gamma^2-1)^\ell\binom{n}{2\ell}\frac{(2\ell)!}{\ell!}\ H_{n-2\ell}(y),

with γ=2/3\gamma=\sqrt{2/3}. The product of the three expansions is a finite linear combination of products HaHbHcH_a H_b H_c. Titchmarsh’s formula then evaluates every remaining integral:

RHaHbHc ey2 dy={π 2s a! b! c!(sa)!(sb)!(sc)!if a+b+c=2s is even and sa,b,c,0otherwise.\int_{\mathbb{R}}H_a H_b H_c\ e^{-y^2}\ dy = \begin{cases} \dfrac{\sqrt{\pi}\ 2^{s}\ a!\ b!\ c!}{(s-a)!(s-b)!(s-c)!} & \text{if }a+b+c=2s\text{ is even and }s\ge a,b,c,\\ 0 & \text{otherwise.} \end{cases}

The result is a finite triple sum (at most O(ijk)O(ijk) terms, typically far fewer). Combining the prefactors NiNjNk2/3N_i N_j N_k\sqrt{2/3} gives Mi,j,kM^{i,j,k} exactly.

Equivalently, the product of two normalized functions expands in a scaled Hermite basis

ψi(x)ψj(x)=r=0(i+j)/2cr;ij ψi+j2r(2 x),\psi_i(x)\psi_j(x)=\sum_{r=0}^{\lfloor(i+j)/2\rfloor}c_{r;ij}\ \psi_{i+j-2r}(\sqrt{2}\ x),

with explicit coefficients

cr;ij=(1)r2i+j2r+1π(i+j2r)!i! j!(ir)(jr)r! 2rc_{r;ij}=\frac{(-1)^r}{\sqrt{2^{i+j-2r+1}\pi}}\sqrt{\frac{(i+j-2r)!}{i!\ j!}}\binom{i}{r}\binom{j}{r}r!\ 2^{r}

(up to the conventional placement of the 2\sqrt{2} in the argument; cf. [K16]). Then

Mi,j,k=rcr;ijRψi+j2r(2 x) ψk(x) dx,M^{i,j,k}=\sum_{r}c_{r;ij}\int_{\mathbb{R}}\psi_{i+j-2r}(\sqrt{2}\ x)\ \psi_k(x)\ dx,

and each scaled overlap is a 2F1{}_2F_1 (or terminates as a short hypergeometric sum). This is the form best suited to computation.

Γ\Gamma Calculus

By definition [BE85]

ΓH(f,g):=12(H(fg)f Hgg Hf).\Gamma_H(f,g):=\frac12\bigl(H(fg)-f\ Hg-g\ Hf\bigr).

On basis vectors this is already diagonal in the spectrum:

ΓH(ei,ej)=12k(λkλiλj) Mi,j,k ek.\Gamma_H(e^i,e^j)=\frac12\sum_k(\lambda_k-\lambda_i-\lambda_j)\ M^{i,j,k}\ e^k.

Hence

ei,ej=ΓH(ei,ej)12Veiej=12k[(λkλiλj)Mi,j,k+Veiejeˉk dx] ek.\begin{aligned} \langle\nabla e^i,\nabla e^j\rangle &=-\Gamma_H(e^i,e^j)-\frac12 V e^i e^j\\ &=-\frac12\sum_k[(\lambda_k-\lambda_i-\lambda_j)M^{i,j,k} +\int V e^i e^j \bar e^k\ dx]\ e^k. \end{aligned}

Ground-state conjugation repairs the VV defect: if Hψ=λ0ψH\psi=\lambda_0\psi with ψ>0\psi>0, then

L:=ψ1(Hλ0)(ψ  )=Δ2logψ,  L:=\psi^{-1}(H-\lambda_0)(\psi\ \cdot\ )=-\Delta-2\langle\nabla\log\psi,\nabla\ \cdot\ \rangle

is a diffusion, and its Bakry–Émery tensor is Ric2Hesslogψ\operatorname{Ric}-2\operatorname{Hess}\log\psi. For the harmonic oscillator the ground state is a Gaussian, logψ0=x2/2+const\log\psi_0=-x^2/2+\mathrm{const}, and one recovers exactly BE(2,)\mathrm{BE}(2,\infty) for this renormalized Ornstein–Uhlenbeck process — the classical diffusion underneath the quantum oscillator.

With ϕ=2logψ0\phi = -2 \log \psi_0 and vwv\cdot w the Riemannian inner product on the cotangent bundle, let us write these operators in the eigenbasis of LL:

fn=ψnψ0,MLi,j,k=ψiψjψkψ0 dvol,ΓL(fi,fj):=12k(λk+λ0λiλj)MLi,j,k fk=dfidfj,Γ2,L(fi,fj):=14k(λk+λ0λiλj)2MLi,j,k fk    Γ2,L(f)=HessfHS2+Ric(f,f)+Hessϕ(f,f).f_n=\frac{\psi_n}{\psi_0},\qquad M_L^{i,j,k}=\int\frac{\psi_i\psi_j\psi_k}{\psi_0}\ d\mathrm{vol},\\ \begin{aligned} \Gamma_L(f_i,f_j):&=\frac12\sum_k(\lambda_k+\lambda_0-\lambda_i-\lambda_j)M_L^{i,j,k}\ f_k = -df_i \cdot df_j,\\ \Gamma_{2,L}(f_i,f_j):&=\frac14\sum_k(\lambda_k+\lambda_0-\lambda_i-\lambda_j)^2 M_L^{i,j,k}\ f_k\implies\\ \Gamma_{2,L}(f)&=\lvert\operatorname{Hess}f\rvert_{\mathrm{HS}}^2+\operatorname{Ric}(\nabla f,\nabla f) + \operatorname{Hess}\phi(\nabla f, \nabla f). \end{aligned}

For a confining Schrödinger operator as in the Theorem, the isometric type of (M,g,V)(M,g,V) is encoded in the diffusion data (λnλ0,MLi,j,k)({\lambda_n-\lambda_0},{M_L^{i,j,k}}), because ΓL\Gamma_L is the cometric and ψ0\psi_0 recovers VV by Riccati.

Returning to Harmonic Oscillator Example

With fn=ψn/ψ0f_n=\psi_n/\psi_0 and dμ=ψ02 dxd\mu=\psi_0^2\ dx,

MLi,j,k=Rψiψjψkψ0 dx=NiNjNkN0HiHjHk ex2 dx.M_L^{i,j,k}=\int_{\mathbb{R}}\frac{\psi_i\psi_j\psi_k}{\psi_0}\ dx=\frac{N_i N_j N_k}{N_0}\int H_i H_j H_k\ e^{-x^2}\ dx.

Titchmarsh then collapses to

MLi,j,k=i! j! k!(si)!(sj)!(sk)!when i+j+k=2s and si,j,k,M_L^{i,j,k} = \frac{\sqrt{i!\ j!\ k!}}{(s-i)!(s-j)!(s-k)!} \quad\text{when }i+j+k=2s\text{ and }s\ge i,j,k,

and 00 otherwise. In particular ML0,n,n=1M_L^{0,n,n}=1, which is orthonormality of ψn{\psi_n} in L2(dx)L^2(dx).

As these structure constants are non-negative on a multiplicity-1 spectrum, they are the associated singular-value invariants [JS24] for LL.