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Nonlocal Modular Hamiltonians and Limits of Explicit Control

Outside exceptional vacuum wedges, conformal balls, and a few other symmetric settings, a modular generator is generally state dependent and nonlocal. “Known perturbatively” is therefore meaningful only after naming a regulator, an operator domain, a small parameter, an error metric, and the spectral region on which the estimate remains finite.

Required background. Spectra and projectors supply finite spectral decompositions, and modular Hamiltonian domains supplies the continuum logarithm.

Helpful background. Shape dependence supplies controlled geometric perturbations.

The chapter overview places these approximations in the route from standard pairs to geometric flow, compares representative modular flows and their boundaries, and gives a checklist for deciding when a modular-flow claim is licensed.

With a UV regulator or a split inclusion, a region may have a density matrix and

KA=−log⁡ρA.K_A=-\log\rho_A.

In an unregulated continuum QFT, a sharp local algebra is typically type III and has no trace-class ρA\rho_A. The intrinsic object is the modular operator ΔA,Ω\Delta_{A,\Omega} in a standard representation, with generator −log⁡ΔA,Ω-\log\Delta_{A,\Omega}. A regulated one-sided expression is useful only if its relation to that algebraic object and its cutoff dependence are stated.

In a regulated operator basis, spatial nonlocality may appear as

KA=∫Add−1x  fμ(x)T0μ(x)+∫Add−1x dd−1y  hab(x,y)Oa(x)Ob(y)+higher multilocal terms.(1)\begin{aligned} K_A={}& \int_A d^{d-1}x\;f^\mu(x)T_{0\mu}(x)\\ &+\int_A d^{d-1}x\,d^{d-1}y\; h_{ab}(x,y)\mathcal O_a(x)\mathcal O_b(y) +\text{higher multilocal terms}. \tag{1} \end{aligned}

The split into local, bilocal, and higher terms depends on the regulated operator basis. What is basis independent is that the adjoint flow need not act as a pointwise spacetime transformation.

Gaussian free fermions: conventions and support

Section titled “Gaussian free fermions: conventions and support”

For a gauge-invariant, number-conserving fermionic Gaussian state, define the one-particle correlation matrix by

Cij=⟨cj†ci⟩.(2)C_{ij}=\langle c_j^\dagger c_i\rangle. \tag{2}

If 0<C<10<C<\mathbf1 on the retained one-particle space, then

KA=∑i,jci†hijcj+c0,h=log⁡ ⁣[(1−C)C−1].(3)K_A=\sum_{i,j}c_i^\dagger h_{ij}c_j+c_0, \qquad h=\log\!\left[(\mathbf1-C)C^{-1}\right]. \tag{3}

This index order matters. Peschel instead writes C~ij=⟨ci†cj⟩=Cji\widetilde C_{ij}=\langle c_i^\dagger c_j\rangle=C_{ji}; in that convention the corresponding statement is

hT=log⁡ ⁣[(1−C~)C~−1],h^{\mathsf T} =\log\!\left[(\mathbf1-\widetilde C)\widetilde C^{-1}\right],

as in Peschel 2003, equations (11)–(12). Omitting the transpose is harmless for a real symmetric correlator but wrong in a general complex basis.

If CC has eigenvalue 00 or 11, (3) is an unbounded limit. One must restrict to the support on which 0<C<10<C<1 or retain the divergent entanglement energies explicitly. If anomalous correlators

Fij=⟨cicj⟩F_{ij}=\langle c_i c_j\rangle

are nonzero, (3) is incomplete: the quadratic generator includes pairing terms and is determined by a Nambu or Majorana covariance matrix Peschel 2003, equations (13)–(15).

Let a faithful regulated state vary as ρ(λ)=ρ0+λ δρ+O(λ2)\rho(\lambda)=\rho_0+\lambda\,\delta\rho+O(\lambda^2). The Fréchet derivative of K=−log⁡ρK=-\log\rho is

δK=−∫0∞dβ  (ρ0+β)−1δρ(ρ0+β)−1.(4)\delta K =-\int_0^\infty d\beta\; (\rho_0+\beta)^{-1}\delta\rho (\rho_0+\beta)^{-1}. \tag{4}

In an eigenbasis ρ0∣m⟩=pm∣m⟩\rho_0|m\rangle=p_m|m\rangle,

(δK)mn=−log⁡pm−log⁡pnpm−pn(δρ)mn,(5)(\delta K)_{mn} =-\frac{\log p_m-\log p_n}{p_m-p_n} (\delta\rho)_{mn}, \tag{5}

with coincident limit −(δρ)nn/pn-(\delta\rho)_{nn}/p_n. Equations (4)–(5) are the standard resolvent and divided-difference forms of a matrix-function derivative Higham 2008, §3.2, especially equations (3.11)–(3.16).

If pmin⁡=min⁡spec⁡ρ0>0p_{\min}=\min\operatorname{spec}\rho_0>0, the operator norm obeys

∥δK∥2≤∥δρ∥2∫0∞dβ(pmin⁡+β)2=∥δρ∥2pmin⁡.(6)\|\delta K\|_2 \le \|\delta\rho\|_2 \int_0^\infty\frac{d\beta}{(p_{\min}+\beta)^2} =\frac{\|\delta\rho\|_2}{p_{\min}}. \tag{6}

The estimate is explicit and reproducible, but its ceiling diverges as pmin⁡→0p_{\min}\to0. This bound therefore supplies no uniform operator-norm control in a continuum or large-volume limit. Such a limit needs either a sharper operator-norm estimate or a declared weaker topology—often matrix elements on an energy-bounded domain, quadratic forms, or modular-frequency-smeared correlators.

Formal modular-time expansions are not automatically controlled

Section titled “Formal modular-time expansions are not automatically controlled”

The logarithm can also be organized as integrals of perturbations transported by a reference modular flow. Schematically,

δK=∫−∞∞ds  g(s) σs(0)(δX),(7)\delta K =\int_{-\infty}^{\infty}ds\; g(s)\,\sigma_s^{(0)}(\delta X), \tag{7}

where the distribution gg and the zero-modular-frequency term depend on the preparation and convention. Contact prescriptions, the sign of modular time, and Fourier normalization must be fixed before two forms of (7) can be compared.

The excited-state series of Sárosi and Ugajin is explicitly presented as a formal expansion, not a convergent expansion for arbitrary states Sárosi–Ugajin 2018, abstract and §2. Their §6 identifies settings that may supply control—small subsystems, large-NN counting subject to multitrace caveats, or a small mixture parameter—but each application must still bound its own remainder Sárosi–Ugajin 2018, §6. Formal modular ordering alone supplies no universal error bar.

For a small deformation ζμ\zeta^\mu of a vacuum half-space, a concrete QFT benchmark is

UKAU†=KA0−2π∫H+ζ+T+++2π∫H−ζ−T−−+2π∫A0ζν[KA0,T0ν]+O(ζ2),(8)\begin{aligned} UK_AU^\dagger={}&K_{A_0} -2\pi\int_{\mathcal H_+}\zeta^+T_{++} +2\pi\int_{\mathcal H_-}\zeta^-T_{--}\\ &+2\pi\int_{A_0}\zeta^\nu [K_{A_0},T_{0\nu}] +O(\zeta^2), \tag{8} \end{aligned}

where UU identifies the deformed and undeformed regulated Hilbert spaces. Equation (8), including its inward-deformation convention, is Faulkner–Leigh–Parrikar–Wang 2016, §1.1, equations (12)–(14). It controls only first order, and the source explains the entangling-surface cutoff in Appendix A. It does not license replacing a generic modular Hamiltonian by a local stress-tensor integral.

First application: a reproducible free-field benchmark

Section titled “First application: a reproducible free-field benchmark”

Use a number-conserving free-fermion regulator and retain two normalized wave-packet modes supported in the deformed region. Suppose the computed restricted correlator is

C(ε)=(1/4εε3/4),r(ε)=116+ε2.(9)C(\varepsilon)= \begin{pmatrix} 1/4&\varepsilon\\ \varepsilon&3/4 \end{pmatrix}, \qquad r(\varepsilon)=\sqrt{\frac1{16}+\varepsilon^2}. \tag{9}

Here ε\varepsilon is the dimensionless first-order response of the two retained modes to the deformation. This benchmark begins after the geometric calculation has supplied (9); it tests the logarithm and modular flow without pretending that every deformation has this two-mode response.

The eigenvalues of CC are 1/2±r1/2\pm r. Faithfulness of both CC and 1−C1-C requires

∣ε∣<34≈0.433013.(10)|\varepsilon|<\frac{\sqrt3}{4}\approx0.433013. \tag{10}

Define

L(ε)=log⁡1/2+r1/2−r.L(\varepsilon) =\log\frac{1/2+r}{1/2-r}.

With σx,σz\sigma_x,\sigma_z the Pauli matrices, exact functional calculus gives

h(ε)=L4r σz−Lεr σx.(11)h(\varepsilon) =\frac{L}{4r}\,\sigma_z -\frac{L\varepsilon}{r}\,\sigma_x. \tag{11}

The first-order approximation is

h(1)(ε)=log⁡3 σz−4εlog⁡3 σx.(12)h^{(1)}(\varepsilon) =\log3\,\sigma_z -4\varepsilon\log3\,\sigma_x. \tag{12}

Thus the first nonlocal correction is the hopping term

δK(1)=−4εlog⁡3 (c1†c2+c2†c1).(13)\delta K^{(1)} =-4\varepsilon\log3\, (c_1^\dagger c_2+c_2^\dagger c_1). \tag{13}

Use the spectral-norm remainder

Rh(ε)=∥h(ε)−h(1)(ε)∥2=(L4r−log⁡3)2+(−Lεr+4εlog⁡3)2.(14)R_h(\varepsilon) =\|h(\varepsilon)-h^{(1)}(\varepsilon)\|_2 =\sqrt{ \left(\frac{L}{4r}-\log3\right)^2 +\left(-\frac{L\varepsilon}{r} +4\varepsilon\log3\right)^2 }. \tag{14}

The benchmark values below follow directly from (9)–(14); “relative remainder” means Rh/(4∣ε∣log⁡3)R_h/(4|\varepsilon|\log3), the remainder divided by the norm of the retained nonlocal correction.

εSmallest eigenvalue of C or 1 − CRemainder normRelative remainder
0.020.2492010.0007540.00858
0.050.2450490.0048250.02196
0.100.2307420.0208860.04753
0.200.1798440.1104960.12572
0.400.0283011.4632930.83247

For a normalized one-particle smearing f∈C2f\in\mathbb C^2, set c(f)=∑ifi∗cic(f)=\sum_i f_i^*c_i. The CAR give ∥c(f)∥=∥f∥2\|c(f)\|=\|f\|_2 and

[K,c(f)]=−c(hf).[K,c(f)]=-c(hf).

Consequently,

∥[K−K(1),c(f)]∥≤Rh∥f∥2,(15)\|[K-K^{(1)},c(f)]\| \le R_h\|f\|_2, \tag{15}

and the exact and truncated modular flows satisfy the Duhamel bound

∥σs(c(f))−σs(1)(c(f))∥≤∣s∣Rh∥f∥2.(16)\|\sigma_s(c(f))-\sigma_s^{(1)}(c(f))\| \le |s|R_h\|f\|_2. \tag{16}

Equations (14)–(16) state the domain, norm, deformation parameter, and modular-time dependence explicitly. No continuum claim is being made: the result controls only these two retained modes at the chosen regulator.

Adversarial test: drive the spectrum to its support boundary

Section titled “Adversarial test: drive the spectrum to its support boundary”

Increasing ∣ε∣|\varepsilon| in (9) simultaneously strengthens the nonlocal coupling and worsens spectral conditioning. At ∣ε∣=3/4|\varepsilon|=\sqrt3/4, the smallest eigenvalue reaches zero, L(ε)L(\varepsilon) diverges, and neither (11) nor the operator-norm estimate has a finite full-space limit. Beyond that point CC is not a valid fermionic correlation matrix because an eigenvalue lies outside [0,1][0,1].

The table shows that the first-order approximation is already poor at ε=0.40\varepsilon=0.40: its remainder is about 83%83\% of the retained correction. The strongest surviving statements are the exact finite-mode formula (11) for the open interval (10), and possibly matrix-element statements on a restricted support. The perturbative claim (12)–(16) must be withdrawn when the chosen tolerance is exceeded; ultraviolet refinement requires a separate convergence study rather than extrapolation from this table.

A publication-level nonlocal calculation should report separately:

  • state or shape truncation: omitted powers of the declared small parameter;
  • spectral conditioning: distance of CC, ρ\rho, or Δ\Delta from its support boundary;
  • operator truncation: omitted bilocal, pairing, or higher multilocal structures;
  • regulator removal: stability under lattice spacing, split distance, volume, and mode-cutoff refinement.

Agreement with entropy alone is not a flow test: an operator with zero expectation value can leave the entropy unchanged while changing commutators and modular evolution.

Using the wrong Gaussian index convention. With Cij=⟨cj†ci⟩C_{ij}=\langle c_j^\dagger c_i\rangle, equation (3) has no transpose. With Peschel’s reversed indices, it does.

Calling a formal modular-time series controlled. Name the regime that suppresses higher orders and exhibit a remainder in the topology actually used.

Keeping an operator-norm claim as the support gap closes. Equations (6) and (14) display the divergence. Change the domain or topology, or stop the claim.

1. Derive the transpose in Peschel’s convention

Section titled “1. Derive the transpose in Peschel’s convention”

Diagonalize a Hermitian one-particle matrix hh and prove that

C~ij=⟨ci†cj⟩\widetilde C_{ij}=\langle c_i^\dagger c_j\rangle

obeys hT=log⁡[(1−C~)C~−1]h^{\mathsf T}=\log[(1-\widetilde C)\widetilde C^{-1}].

Solution

Write h=UϵU†h=U\epsilon U^\dagger and ci=∑αUiαdαc_i=\sum_\alpha U_{i\alpha}d_\alpha. For the Gaussian density operator proportional to e−c†hce^{-c^\dagger hc},

⟨dα†dβ⟩=δαβ11+eϵα.\langle d_\alpha^\dagger d_\beta\rangle =\delta_{\alpha\beta}\frac1{1+e^{\epsilon_\alpha}}.

Therefore

C~ij=∑αUiα∗Ujα11+eϵα=[(1+eh)−1]ji.\widetilde C_{ij} =\sum_\alpha U_{i\alpha}^*U_{j\alpha} \frac1{1+e^{\epsilon_\alpha}} =\left[(1+e^h)^{-1}\right]_{ji}.

In matrix notation,

C~T=(1+eh)−1.\widetilde C^{\mathsf T}=(1+e^h)^{-1}.

Solving for hh gives

h=log⁡[(1−C~T)(C~T)−1],h=\log[(1-\widetilde C^{\mathsf T}) (\widetilde C^{\mathsf T})^{-1}],

and transposing yields the claimed formula. For complex UU, dropping the transpose changes the matrix; it is not merely notation.

Starting from (4), prove (6) and state exactly why it gives no uniform continuum estimate when pmin⁡→0p_{\min}\to0.

Solution

Because ρ0≥pmin⁡1\rho_0\ge p_{\min}\mathbf1,

∥(ρ0+β)−1∥2≤1pmin⁡+β.\|(\rho_0+\beta)^{-1}\|_2 \le\frac1{p_{\min}+\beta}.

Submultiplicativity and (4) give

∥δK∥2≤∥δρ∥2∫0∞dβ(pmin⁡+β)2=∥δρ∥2pmin⁡.\|\delta K\|_2 \le\|\delta\rho\|_2 \int_0^\infty\frac{d\beta}{(p_{\min}+\beta)^2} =\frac{\|\delta\rho\|_2}{p_{\min}}.

If a regulator sequence has pmin⁡→0p_{\min}\to0, the right-hand side diverges even when ∥δρ∥2\|\delta\rho\|_2 stays fixed. Hence the estimate supplies no regulator-independent operator-norm control. A weaker, explicitly declared topology may still converge, but that is a different claim requiring its own proof.

3. Reproduce the two-mode error and flow bound

Section titled “3. Reproduce the two-mode error and flow bound”

At ε=0.10\varepsilon=0.10, compute rr, the support gap, LL, and RhR_h. Then bound the flow error at ∣s∣=2|s|=2 for ∥f∥2=1\|f\|_2=1.

Solution

Equations (9)–(11) give

r=0.0625+0.01=0.269258,pgap=0.5−r=0.230742,r=\sqrt{0.0625+0.01}=0.269258, \qquad p_{\rm gap}=0.5-r=0.230742,

and

L=log⁡0.7692580.230742=1.204128.L=\log\frac{0.769258}{0.230742}=1.204128.

Substitution in (14) gives

Rh=0.020886.R_h=0.020886.

The commutator error for a normalized smearing is at most 0.0208860.020886. Equation (16) gives

∥σs(c(f))−σs(1)(c(f))∥≤2Rh=0.041772\|\sigma_s(c(f))-\sigma_s^{(1)}(c(f))\| \le2R_h =0.041772

at ∣s∣=2|s|=2. This is a finite-mode operator-norm statement; it does not bound omitted regulator modes or the O(ζ2)O(\zeta^2) geometric remainder that led to the input correlator.

  • Faulkner, Thomas, Robert G. Leigh, Onkar Parrikar, and Huajia Wang. “Modular Hamiltonians for Deformed Half-Spaces and the Averaged Null Energy Condition.” Journal of High Energy Physics 2016, no. 9 (2016): 038. DOI. Open HTML, equations (12)–(14).
  • Higham, Nicholas J. Functions of Matrices: Theory and Computation. Philadelphia: Society for Industrial and Applied Mathematics, 2008. DOI.
  • Peschel, Ingo. “Calculation of Reduced Density Matrices from Correlation Functions.” Journal of Physics A: Mathematical and General 36 (2003): L205–L208. DOI. Open preprint.
  • Sárosi, Gábor, and Tomonori Ugajin. “Modular Hamiltonians of Excited States, OPE Blocks and Emergent Bulk Fields.” Journal of High Energy Physics 2018, no. 1 (2018): 012. DOI. Open HTML.

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