Skip to content

Modular Spectrum and Spectral Measures

Finite density matrices turn modular spectra into ratios of probabilities. A continuum algebra need not retain a countable list of levels: the useful object may instead be a projection-valued measure, a vector spectral measure, or a state-independent factor invariant. These objects must be kept distinct, and continuity or type-III1_1 behavior must be proved from a limiting construction or a structural theorem rather than inferred from a dense finite plot.

Required background. Modular Hamiltonian definitions and domains supply the support compression, logarithmic functional calculus, and unbounded-operator domains used here.

Helpful background. Tomita–Takesaki flow supplies the standard pair, modular conjugation, and invariant vector used to derive reciprocal spectral symmetry.

The chapter’s route from standard pairs to geometric flow identifies which spectra are intrinsic. The representative-flow table separates exact continuum objects from regulated representatives, and the claim-licensing checklist tests any proposed continuum inference.

Let (A,Ω)(\mathcal A,\Omega) be standard and let Δ\Delta be its modular operator. Then Δ\Delta is positive, self-adjoint, and injective. Injectivity means EΔ({0})=0E_\Delta(\{0\})=0; it does not prevent 00 from belonging to the continuous spectrum. The spectral theorem gives

Δ=∫[0,∞)λ EΔ(dλ),K=−log⁡Δ=∫Rk EK(dk),\Delta=\int_{[0,\infty)}\lambda\,E_\Delta(d\lambda), \qquad K=-\log\Delta =\int_{\mathbb R}k\,E_K(dk),

where k=−log⁡λk=-\log\lambda on λ>0\lambda>0. For a vector ξ\xi,

μξK(B)=⟨ξ,EK(B)ξ⟩\mu_\xi^K(B)=\langle\xi,E_K(B)\xi\rangle

is a finite positive measure, and it is a probability measure only when ∥ξ∥=1\lVert\xi\rVert=1. The exact domain test for a Borel function is

ξ∈D(f(K))⟺∫R∣f(k)∣2dμξK(k)<∞.\xi\in\mathcal D(f(K)) \quad\Longleftrightarrow\quad \int_{\mathbb R}\lvert f(k)\rvert^2d\mu_\xi^K(k)<\infty.

Cross measures

μξ,ηK(B)=⟨ξ,EK(B)η⟩\mu_{\xi,\eta}^K(B)=\langle\xi,E_K(B)\eta\rangle

are generally complex. They encode modular correlators, but they are not probability distributions. The invariant vector satisfies KΩ=0K\Omega=0; this gives one zero eigenvector without making zero isolated or supplying an eigenbasis for the rest of the Hilbert space.

If a normal state is not faithful, first compress to its support projection p=s(ω)p=s(\omega) and work with pApp\mathcal A p. In a type-I model this means discarding the zero eigenspace before taking log⁡ρ\log\rho. Writing an infinite “entanglement energy” for every vector in the discarded kernel is regulator notation, not the spectral calculus of a standard faithful pair.

Reciprocal symmetry and finite ratio spectra

Section titled “Reciprocal symmetry and finite ratio spectra”

Tomita–Takesaki theory gives

JΔJ=Δ−1,JKJ=−K.J\Delta J=\Delta^{-1}, \qquad JKJ=-K.

Hence

0<λ∈spec⁡(Δ)⟺λ−1∈spec⁡(Δ),k∈spec⁡(K)⟺−k∈spec⁡(K),0<\lambda\in\operatorname{spec}(\Delta) \Longleftrightarrow \lambda^{-1}\in\operatorname{spec}(\Delta), \qquad k\in\operatorname{spec}(K) \Longleftrightarrow -k\in\operatorname{spec}(K),

and, for every Borel set B⊂RB\subset\mathbb R,

JEK(B)J=EK(−B),μJξK(B)=μξK(−B).J E_K(B)J=E_K(-B), \qquad \mu_{J\xi}^K(B)=\mu_\xi^K(-B).

The measure of a generic ξ\xi need not be even: the reflected measure belongs to JξJ\xi.

For a faithful finite density matrix ρ=∑ipi∣i⟩⟨i∣\rho=\sum_i p_i\lvert i\rangle\langle i\rvert, use the Hilbert–Schmidt standard representation. Matrix units obey

Δ(∣i⟩⟨j∣)=pipj∣i⟩⟨j∣,K(∣i⟩⟨j∣)=−log⁡ ⁣pipj∣i⟩⟨j∣.\Delta(\lvert i\rangle\langle j\rvert) =\frac{p_i}{p_j}\lvert i\rangle\langle j\rvert, \qquad K(\lvert i\rangle\langle j\rvert) =-\log\!\frac{p_i}{p_j}\lvert i\rangle\langle j\rvert.

The standard modular spectrum is therefore a ratio set. The one-sided entanglement levels −log⁡pi-\log p_i are different data; only their pairwise differences occur as eigenvalues of KK. Multiplicity in the standard representation also differs from multiplicity in the one-sided density matrix.

One state’s spectrum versus the Connes invariant

Section titled “One state’s spectrum versus the Connes invariant”

The Connes SS-invariant of a von Neumann algebra is not the spectrum of one chosen modular operator. In its weight formulation,

S(M)=⋂φspec⁡(Δφ),S(\mathcal M) =\bigcap_{\varphi} \operatorname{spec}(\Delta_\varphi),

where the intersection is over faithful normal semifinite weights in the standard construction. Connes gives this definition in Connes 1973, Definition 3.1.1, printed p. 188. For type-III factors, the resulting classification is

factorS(M)S(\mathcal M)
III0\mathrm{III}_0{0,1}\{0,1\}
IIIλ\mathrm{III}_\lambda, 0<λ<10<\lambda<1{0}∪{λn:n∈Z}\{0\}\cup\{\lambda^n:n\in\mathbb Z\}
III1\mathrm{III}_1[0,∞)[0,\infty)

These cases appear at the opening of Connes 1973, Part IV, printed p. 214. The zero in S(M)S(\mathcal M) is a spectral boundary point; injective modular operators still have no zero eigenvector.

This distinction also limits QFT claims. Fredenhagen proves full positive modular spectra, and hence type-III1_1 central components, for local algebras under an asymptotic scale-invariance hypothesis Fredenhagen 1985, abstract and pp. 79–89. That result does not license the sentence “every continuum local algebra is type III1_1” without the model’s locality, standardness, scaling, and factoriality hypotheses. Nor does type III1_1 imply that every chosen vector measure is absolutely continuous.

A finite Gaussian sequence for a free wedge

Section titled “A finite Gaussian sequence for a free wedge”

The free wedge supplies a concrete continuous target. In rapidity variables, longitudinal boosts act by translations, so the one-particle boost generator has continuous spectrum on R\mathbb R. The Bisognano–Wichmann theorem fixes the wedge modular generator to 2π2\pi times that boost generator, with orientation set by convention Bisognano and Wichmann 1976, §III, pp. 306–310.

Consider a free-fermion spectral Galerkin model. Choose a cutoff LL, spacing δ\delta, and midpoint grid

kj=−L+(j+12)δ,j=0,…,N−1,N=2Lδ.k_j=-L+\left(j+\frac12\right)\delta, \qquad j=0,\ldots,N-1, \qquad N=\frac{2L}{\delta}.

Define the one-particle Gaussian modular matrix and correlation matrix by

hδ,L=diag⁡(kj),Cδ,L=(I+ehδ,L)−1.h_{\delta,L}=\operatorname{diag}(k_j), \qquad C_{\delta,L}=\left(I+e^{h_{\delta,L}}\right)^{-1}.

Thus every eigenvalue of CC lies strictly between zero and one and

hδ,L=log⁡ ⁣[(I−Cδ,L)Cδ,L−1].h_{\delta,L} =\log\!\left[(I-C_{\delta,L})C_{\delta,L}^{-1}\right].

This is the number-conserving Gaussian reconstruction derived in Peschel 2003, Eqs. (5)–(12), printed pp. L205–L206; a transpose appears in Peschel’s site-index convention and is immaterial in this diagonal basis.

Let Hδ,L=∑jkjcj†cjH_{\delta,L}=\sum_j k_jc_j^\dagger c_j and ρδ,L=Z−1e−Hδ,L\rho_{\delta,L}=Z^{-1}e^{-H_{\delta,L}}. In Hilbert–Schmidt standard form,

Kδ,L(X)=Hδ,LX−XHδ,L.K_{\delta,L}(X)=H_{\delta,L}X-XH_{\delta,L}.

If ∣0⟩\lvert0\rangle is the Fock vacuum and ∣j⟩=cj†∣0⟩\lvert j\rangle=c_j^\dagger\lvert0\rangle, then Xj=∣j⟩⟨0∣X_j=\lvert j\rangle\langle0\rvert has modular eigenvalue kjk_j. Choose

ξδ,L=∑jwj Xj,wj=δe−kj2/2∑ℓδe−kℓ2/2.\xi_{\delta,L}=\sum_j\sqrt{w_j}\,X_j, \qquad w_j= \frac{\delta e^{-k_j^2/2}} {\sum_\ell\delta e^{-k_\ell^2/2}}.

Its exact vector spectral measure and characteristic function are

μδ,LK=∑jwjδkj,χδ,L(s)=∑jwje−iskj.\mu_{\delta,L}^K=\sum_jw_j\delta_{k_j}, \qquad \chi_{\delta,L}(s)=\sum_jw_je^{-isk_j}.

In the joint limit δ↓0\delta\downarrow0, L↑∞L\uparrow\infty, these Riemann sums converge weakly to the selected continuum boost-frequency wavepacket

dμ(k)=e−k2/22π dk,χ(s)=e−s2/2.d\mu(k)=\frac{e^{-k^2/2}}{\sqrt{2\pi}}\,dk, \qquad \chi(s)=e^{-s^2/2}.

This is a vector-measure convergence test for a one-particle free-wedge sector. It is not a proof that a particular spatial lattice recovers the full wedge algebra, its spectral multiplicity, or its Connes invariant.

For reproduction, use midpoint sums in double precision and the sample set S={0.5,1,2}\mathcal S=\{0.5,1,2\}. Separate grid and full-target errors:

Egrid=max⁡s∈S∣χδ,L(s)−χδ/2,L(s)∣,Efull=max⁡s∈S∣χδ,L(s)−e−s2/2∣.\begin{aligned} E_{\mathrm{grid}}&= \max_{s\in\mathcal S} \lvert\chi_{\delta,L}(s)-\chi_{\delta/2,L}(s)\rvert,\\ E_{\mathrm{full}}&= \max_{s\in\mathcal S} \lvert\chi_{\delta,L}(s)-e^{-s^2/2}\rvert. \end{aligned}
LLδ\deltaNNEgridE_{\mathrm{grid}}EfullE_{\mathrm{full}}
440.5000.50016161.05×10−51.05\times10^{-5}7.61×10−57.61\times10^{-5}
440.2500.25032322.92×10−62.92\times10^{-6}8.51×10−58.51\times10^{-5}
440.1250.12564647.51×10−77.51\times10^{-7}8.75×10−58.75\times10^{-5}
220.1250.12532321.72×10−41.72\times10^{-4}6.09×10−26.09\times10^{-2}
550.1250.12580801.17×10−81.17\times10^{-8}9.78×10−79.78\times10^{-7}

At fixed L=4L=4, refinement reduces the grid error while exposing the nonzero window bias; increasing LL then removes that bias. The displayed digits are rounded from the stated sums, so the last quoted digit carries ordinary floating-point and rounding uncertainty.

The L=2L=2 row is an intentional failure. Shrinking only the energy window increases EfullE_{\mathrm{full}} from 8.75×10−58.75\times10^{-5} to 6.09×10−26.09\times10^{-2} at the same δ=0.125\delta=0.125. The finite measure now has an artificial band edge at ∣k∣=2\lvert k\rvert=2; it cannot establish a gap or compact support in the continuum target.

Grid placement can manufacture an apparent zero mode. The midpoint grid has smallest reported ∣kj∣=δ/2\lvert k_j\rvert=\delta/2, whereas a node-centered grid contains k=0k=0. At L=4L=4 and δ=0.125\delta=0.125, the maximum difference of their characteristic functions on S\mathcal S is 1.93×10−51.93\times10^{-5}, even though one finite point set appears “gapped” and the other does not. Both converge to the same continuous measure. Apparent point degeneracies and gaps that move under this shift are discretization artifacts.

A pure basis change provides a sharper control: it must change nothing if every object is transported. Take

h=diag⁡(−1,1),ψ=(3/21/2),U=12(111−1).h=\operatorname{diag}(-1,1), \qquad \psi=\begin{pmatrix}\sqrt3/2\\1/2\end{pmatrix}, \qquad U=\frac1{\sqrt2} \begin{pmatrix}1&1\\1&-1\end{pmatrix}.

The original characteristic function is

χ(s)=34eis+14e−is.\chi(s)=\frac34e^{is}+\frac14e^{-is}.

Transporting both h′=UhU∗h'=UhU^* and ψ′=Uψ\psi'=U\psi leaves χ\chi exactly invariant. If one changes the matrix basis but mistakenly keeps the old coordinate vector ψ\psi, the new spectral weights are (2±3)/4(2\pm\sqrt3)/4. At s=π/2s=\pi/2 the wrong answer is i3/2i\sqrt3/2 instead of i/2i/2, an absolute residual

Rbasis=3−12=0.3660254….R_{\mathrm{basis}}=\frac{\sqrt3-1}{2}=0.3660254\ldots.

For genuinely different truncation subspaces there is no exact invariance; report the projection, window, grid placement, vector transport, and convergence of measures or resolvents. A finite eigenvalue list alone cannot decide continuum spectral type.

For normalized ξ\xi,

Cξ(s)=⟨ξ,e−isKξ⟩=∫Re−iskdμξK(k)C_\xi(s)=\langle\xi,e^{-isK}\xi\rangle =\int_{\mathbb R}e^{-isk}d\mu_\xi^K(k)

is positive definite, and its Fourier transform reconstructs the measure in the distributional sense. A finite time window multiplies CξC_\xi and therefore convolves the spectral measure with the transform of that window. Report the time range, sampling interval, window function, nominal frequency resolution, positivity residual, and any KMS detailed-balance residual.

Unitary equivalence preserves spectral data only covariantly:

K′=UKU∗,EK′(B)=UEK(B)U∗,μUξK′=μξK.K'=UKU^*, \qquad E_{K'}(B)=UE_K(B)U^*, \qquad \mu_{U\xi}^{K'}=\mu_\xi^K.

Changing the state or algebra constructs a different modular operator. Restricting to a subalgebra is not “deleting levels,” and a UV regulator is not generally a unitary change of representation.

Equating one-sided levels with standard modular eigenvalues. The levels −log⁡pi-\log p_i and the differences −log⁡(pi/pj)-\log(p_i/p_j) answer different questions and have different multiplicities.

Reading continuum spectral type from finite eigenvalues. Every finite matrix has pure point spectrum. Establish a joint cutoff limit of measures, correlators, or resolvents before calling a limit continuous or gapped.

Using S(M)S(\mathcal M) as another name for spec⁡(ΔΩ)\operatorname{spec}(\Delta_\Omega). The former is an intersection over modular data; the latter depends on one algebra–state pair. State which object was computed.

1. Ratio spectrum, multiplicity, and support

Section titled “1. Ratio spectrum, multiplicity, and support”

Let ρ=diag⁡(1/2,1/3,1/6)\rho=\operatorname{diag}(1/2,1/3,1/6). Find the spectra of Δ\Delta and KK in Hilbert–Schmidt standard form, including the multiplicity of the eigenvalue 11 of Δ\Delta. Compare with the one-sided entanglement levels. What changes if the last probability is set to zero and the remaining support is renormalized?

Solution

The ratio set is

spec⁡(Δ)={1,32,3,23,2,13,12}.\operatorname{spec}(\Delta) =\left\{1,\frac32,3,\frac23,2,\frac13,\frac12\right\}.

Each diagonal matrix unit ∣i⟩⟨i∣\lvert i\rangle\langle i\rvert has ratio one, so 11 has multiplicity three. All six off-diagonal ordered pairs give the six nonunit ratios above, each once. Therefore

spec⁡(K)={0,−log⁡32,−log⁡3,−log⁡23,−log⁡2,−log⁡13,−log⁡12},\operatorname{spec}(K) =\left\{0,-\log\frac32,-\log3, -\log\frac23,-\log2,-\log\frac13,-\log\frac12\right\},

with zero of multiplicity three. The one-sided levels are

{log⁡2,log⁡3,log⁡6},\{\log2,\log3,\log6\},

and are not the same set; their ordered differences produce the eigenvalues of KK. If the last probability is zero, ρ−1\rho^{-1} and log⁡ρ\log\rho are undefined on that vector. After compression and renormalization the nonzero probabilities are 3/53/5 and 2/52/5; their common normalization cancels from ratios. The faithful support therefore gives {1,3/2,2/3}\{1,3/2,2/3\}, with the unit ratio of multiplicity two. Infinite symbols attached to the discarded direction do not belong to this faithful standard pair.

For the grid construction, prove that h=log⁡[(I−C)C−1]h=\log[(I-C)C^{-1}]. Show that Xj=∣j⟩⟨0∣X_j=\lvert j\rangle\langle0\rvert is an eigenvector of the standard generator, derive χδ,L\chi_{\delta,L}, and evaluate its joint continuum limit.

Solution

Since C=(I+eh)−1C=(I+e^h)^{-1},

I−C=eh(I+eh)−1,(I−C)C−1=eh.I-C=e^h(I+e^h)^{-1}, \qquad (I-C)C^{-1}=e^h.

Functional calculus therefore gives log⁡[(I−C)C−1]=h\log[(I-C)C^{-1}]=h. The Fock vacuum has energy zero and ∣j⟩\lvert j\rangle has energy kjk_j, so

K(Xj)=H∣j⟩⟨0∣−∣j⟩⟨0∣H=kjXj.K(X_j)=H\lvert j\rangle\langle0\rvert -\lvert j\rangle\langle0\rvert H =k_jX_j.

The XjX_j are orthonormal in Hilbert–Schmidt norm. Consequently ξ=∑jwjXj\xi=\sum_j\sqrt{w_j}X_j is normalized and

⟨ξ,e−isKξ⟩=∑jwje−iskj=χδ,L(s).\langle\xi,e^{-isK}\xi\rangle =\sum_jw_je^{-isk_j}=\chi_{\delta,L}(s).

At fixed LL, midpoint Riemann sums converge as δ↓0\delta\downarrow0 to the normalized Gaussian restricted to [−L,L][-L,L]. Sending L↑∞L\uparrow\infty then gives

12π∫−∞∞e−k2/2e−iskdk=e−s2/2.\frac1{\sqrt{2\pi}} \int_{-\infty}^{\infty}e^{-k^2/2}e^{-isk}dk =e^{-s^2/2}.

Pointwise convergence of these characteristic functions, with continuity at s=0s=0, is equivalent to weak convergence of the probability measures.

For the two-mode basis test, compute χ(π/2)\chi(\pi/2) before and after the correctly transported Hadamard rotation. Then keep ψ\psi unrotated, find the wrong spectral weights, and compute the residual. Finally explain why changing LL from 44 to 22 is not a basis change.

Solution

For h=diag⁡(−1,1)h=\operatorname{diag}(-1,1), the weights of ψ\psi are 3/43/4 and 1/41/4, so

χ(π/2)=34i+14(−i)=i2.\chi(\pi/2) =\frac34 i+\frac14(-i)=\frac i2.

If h′=UhU∗h'=UhU^* and ψ′=Uψ\psi'=U\psi, then

⟨ψ′,e−ish′ψ′⟩=⟨ψ,e−ishψ⟩\langle\psi',e^{-ish'}\psi'\rangle =\langle\psi,e^{-ish}\psi\rangle

for every ss. If hh is rotated but the coordinate vector is not, the overlaps with the new eigenvectors give

w−=2+34,w+=2−34.w_-=\frac{2+\sqrt3}{4}, \qquad w_+=\frac{2-\sqrt3}{4}.

Thus χwrong(π/2)=i(w−−w+)=i3/2\chi_{\rm wrong}(\pi/2)=i(w_--w_+)=i\sqrt3/2 and

∣χwrong(π/2)−χ(π/2)∣=3−12.\left\lvert\chi_{\rm wrong}(\pi/2)-\chi(\pi/2)\right\rvert =\frac{\sqrt3-1}{2}.

This is a bookkeeping failure under a unitary equivalence. By contrast, changing LL changes the projected spectral subspace and discards weight; no unitary within the old finite space can restore it. The resulting error must be controlled by increasing the window and checking convergence against the same target measure.

  • Bisognano, Joseph J., and Eyvind H. Wichmann. “On the Duality Condition for Quantum Fields.” Journal of Mathematical Physics 17 (1976): 303–321. DOI.
  • Connes, Alain. “Une classification des facteurs de type III.” Annales Scientifiques de l’École Normale Supérieure 6 (1973): 133–252. DOI; Open PDF.
  • Fredenhagen, Klaus. “On the Modular Structure of Local Algebras of Observables.” Communications in Mathematical Physics 97 (1985): 79–89. DOI.
  • Peschel, Ingo. “Calculation of Reduced Density Matrices from Correlation Functions.” Journal of Physics A: Mathematical and General 36 (2003): L205–L208. DOI; arXiv PDF.

Original QFT.org content:CC BY 4.0, unless an item supplies different terms. Third-party material retains its own terms.