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Quantum Fisher Information in QFT

Quantum Fisher information (QFI) measures the local distinguishability of a normalized state family. This page uses the symmetric logarithmic derivative (SLD): it is operationally tied to optimal measurements, but it is not the relative-entropy Hessian. In QFT the distinction becomes practical because a tangent can have finite SLD QFI while failing the stronger modular-energy domain needed by the Bogoliubov–Kubo–Mori response.

Required background. State perturbations and relative-entropy susceptibility provide normalized tangents and the Hessian convention used for relative entropy.

Helpful background. Operational distinguishability bounds provide the measurement and data-processing interpretation.

The chapter’s differentiable-family starting point fixes the tangent and normalization condition. Its metric comparison then fixes the normalization dictionary, while the independent validity gates separate support, domain, and regulator questions.

Let ρλ\rho_\lambda be a differentiable family of density operators and set X=∂λρλX=\partial_\lambda\rho_\lambda, so Tr⁡X=0\operatorname{Tr}X=0. The SLD LL is defined by

X=12(ρL+Lρ),FSLD(X,X)=Tr⁡(ρL2).X=\frac12(\rho L+L\rho), \qquad F_{\rm SLD}(X,X)=\operatorname{Tr}(\rho L^2).

For a faithful state ρ=∑npn∣n⟩⟨n∣\rho=\sum_n p_n\lvert n\rangle\langle n\rvert,

Lmn=2Xmnpm+pn,FSLD(X,X)=∑m,n2∣Xmn∣2pm+pn.L_{mn}=\frac{2X_{mn}}{p_m+p_n}, \qquad F_{\rm SLD}(X,X) =\sum_{m,n}\frac{2\lvert X_{mn}\rvert^2}{p_m+p_n}.

These formulas use the Petz normalization: a commuting tangent gives the ordinary classical Fisher metric ∑nXnn2/pn\sum_n X_{nn}^2/p_n. At non-full rank, retain only terms with pm+pn>0p_m+p_n>0 for a fixed-support tangent and analyze any support-changing limit separately. A tangent into a vanishing eigenspace can make the metric divergent or discontinuous.

For a normalized pure vector,

FSLD=4(⟨∂λψ∣∂λψ⟩−∣⟨ψ∣∂λψ⟩∣2).F_{\rm SLD} =4\left( \langle\partial_\lambda\psi\mid\partial_\lambda\psi\rangle -\lvert\langle\psi\mid\partial_\lambda\psi\rangle\rvert^2 \right).

The subtraction removes the unobservable phase tangent. For a unitary family ρλ=e−iλGρeiλG\rho_\lambda=e^{-i\lambda G}\rho e^{i\lambda G}, the spectral formula becomes

FSLD=∑m,n2(pm−pn)2pm+pn∣Gmn∣2,F_{\rm SLD} =\sum_{m,n} \frac{2(p_m-p_n)^2}{p_m+p_n}\lvert G_{mn}\rvert^2,

and reduces to 4Var⁡ψ(G)4\operatorname{Var}_\psi(G) on a pure state.

What the measurement statement does and does not say

Section titled “What the measurement statement does and does not say”

A POVM {Mx}\{M_x\} gives p(x∣λ)=Tr⁡(ρλMx)p(x\mid\lambda)=\operatorname{Tr}(\rho_\lambda M_x) and

F{Mx}=∑xp(x∣λ)[∂λlog⁡p(x∣λ)]2.F_{\{M_x\}} =\sum_x p(x\mid\lambda) \left[\partial_\lambda\log p(x\mid\lambda)\right]^2.

For unrestricted measurements in the regular finite-dimensional problem,

F{Mx}≤FSLD,F_{\{M_x\}}\leq F_{\rm SLD},

and an SLD-adapted measurement attains equality locally Braunstein and Caves 1994, Eqs. (2)–(4) and (14)–(16), pp. 3440–3442. “Locally” matters: the measurement may depend on the unknown parameter, and a QFT experiment may allow only a subalgebra or an energy-bounded class of measurements. In that case the accessible Fisher information can be strictly smaller.

For NN independent repetitions and a locally unbiased estimator,

Var⁡(λ^)≥1NFSLD.\operatorname{Var}(\widehat\lambda)\geq\frac{1}{N F_{\rm SLD}}.

Finite samples, bias, nuisance parameters, correlated repetitions, and restricted measurements require their corresponding versions of the bound.

SLD versus relative-entropy Fisher information

Section titled “SLD versus relative-entropy Fisher information”

For a faithful finite state, define the Bogoliubov–Kubo–Mori (BKM) quadratic form by

gBKM(X,X)=∑m,nlog⁡pm−log⁡pnpm−pn∣Xmn∣2,g_{\rm BKM}(X,X) =\sum_{m,n} \frac{\log p_m-\log p_n}{p_m-p_n} \lvert X_{mn}\rvert^2,

where the diagonal quotient is 1/pn1/p_n. It is normalized so that

S(ρ+λX∥ρ)=λ22gBKM(X,X)+O(λ3).S(\rho+\lambda X\Vert\rho) =\frac{\lambda^2}{2}g_{\rm BKM}(X,X)+O(\lambda^3).

The relative-entropy Hessian construction and its monotonicity are developed in Lesniewski and Ruskai 1999, §2.3, Theorems 2.8–2.10. The logarithmic-mean inequality gives, term by term,

2pm+pn≤log⁡pm−log⁡pnpm−pn,\frac{2}{p_m+p_n} \leq \frac{\log p_m-\log p_n}{p_m-p_n},

so

FSLD(X,X)≤gBKM(X,X).F_{\rm SLD}(X,X)\leq g_{\rm BKM}(X,X).

Equality holds for commuting tangents, not for a generic coherent direction. The geometric Bures line element is instead gBures=FSLD/4g_{\rm Bures}=F_{\rm SLD}/4; forgetting this factor of four is a common source of apparently inconsistent formulas.

QFT application: a Gaussian source amplitude

Section titled “QFT application: a Gaussian source amplitude”

Consider a finite box and ultraviolet cutoff, with independent real bosonic modes

[qk,pℓ]=iδkℓ,HΛ=∑k∈KΛωk2(qk2+pk2),ρβ=Z−1e−βHΛ.[q_k,p_\ell]=i\delta_{k\ell}, \qquad H_\Lambda=\sum_{k\in\mathcal K_\Lambda} \frac{\omega_k}{2}(q_k^2+p_k^2), \qquad \rho_\beta=Z^{-1}e^{-\beta H_\Lambda}.

Here qk,pkq_k,p_k are dimensionless oscillator quadratures; the real-mode set KΛ\mathcal K_\Lambda includes each physical oscillator once. Estimate the amplitude λ\lambda of the smeared displacement

ρλ=UλρβUλ†,Uλ=exp⁡ ⁣(−iλ∑kgkpk).\rho_\lambda=U_\lambda\rho_\beta U_\lambda^\dagger, \qquad U_\lambda=\exp\!\left(-i\lambda\sum_k g_kp_k\right).

It shifts ⟨qk⟩\langle q_k\rangle by λgk\lambda g_k. A thermal mode has rk=e−βωkr_k=e^{-\beta\omega_k} and pn,k=(1−rk)rknp_{n,k}=(1-r_k)r_k^n. Since pkp_k connects only nn to n+1n+1, inserting ∣⟨n+1∣pk∣n⟩∣2=(n+1)/2\lvert\langle n+1\lvert p_k\rvert n\rangle\rvert^2=(n+1)/2 into the unitary spectral formula yields

FSLD(Λ)=2∑k∈KΛgk2tanh⁡ ⁣(βωk2).F_{\rm SLD}^{(\Lambda)} =2\sum_{k\in\mathcal K_\Lambda} g_k^2\tanh\!\left(\frac{\beta\omega_k}{2}\right).

The same answer follows from the Gaussian first-moment term in Monras 2013, Eqs. (13) and (16). Because displacement leaves the entropy unchanged,

S(ρλ∥ρ0)=β(⟨HΛ⟩λ−⟨HΛ⟩0)=λ22β∑kωkgk2⏟gBKM(Λ).S(\rho_\lambda\Vert\rho_0) =\beta\bigl(\langle H_\Lambda\rangle_\lambda- \langle H_\Lambda\rangle_0\bigr) =\frac{\lambda^2}{2} \underbrace{\beta\sum_k\omega_kg_k^2}_{g_{\rm BKM}^{(\Lambda)}}.

Thus the two Petz-normalized metrics are

FSLD(Λ)=2∑kgk2tanh⁡(βωk/2),gBKM(Λ)=β∑kωkgk2.F_{\rm SLD}^{(\Lambda)} =2\sum_k g_k^2\tanh(\beta\omega_k/2), \qquad g_{\rm BKM}^{(\Lambda)} =\beta\sum_k\omega_kg_k^2.

The inequality 2tanh⁡(x/2)≤x2\tanh(x/2)\leq x checks the general ordering mode by mode. The benchmark is exact at finite volume and cutoff: there is no statistical or truncation error beyond the declared mode regulator. Its controls are LL, Λ\Lambda, β\beta, the dispersion ωk\omega_k, the real-mode counting convention, and the source coefficients gkg_k.

Adversarial test: an energetic-domain failure

Section titled “Adversarial test: an energetic-domain failure”

Let the high-frequency dispersion be relativistic, ωk∼∣k∣\omega_k\sim\lvert k\rvert, in dsd_s spatial dimensions, and let g(k)∼C∣k∣−αg(k)\sim C\lvert k\rvert^{-\alpha}. At fixed positive temperature, the ultraviolet behaviors are

FSLD(Λ)∼∫Λdk  kds−1−2α,gBKM(Λ)∼β∫Λdk  kds−2α.F_{\rm SLD}^{(\Lambda)} \sim\int^{\Lambda}dk\;k^{d_s-1-2\alpha}, \qquad g_{\rm BKM}^{(\Lambda)} \sim\beta\int^{\Lambda}dk\;k^{d_s-2\alpha}.

Therefore

FSLD<∞  ⟺  2α>ds,gBKM<∞  ⟺  2α>ds+1.F_{\rm SLD}<\infty\iff 2\alpha>d_s, \qquad g_{\rm BKM}<\infty\iff 2\alpha>d_s+1.

Equality at either threshold gives a logarithmic divergence. In the window

ds2<α≤ds+12,\frac{d_s}{2}<\alpha\leq\frac{d_s+1}{2},

the SLD limit exists but the BKM metric and injected energy

ΔEΛ=λ22∑kωkgk2\Delta E_\Lambda =\frac{\lambda^2}{2}\sum_k\omega_kg_k^2

do not. This is the promised failure injection: finite statistical distinguishability alone does not put the source in the Hamiltonian energy domain. For α≤ds/2\alpha\leq d_s/2, even the SLD quantity is only a cutoff-dependent family. A continuum claim must specify smearing strong enough for the intended metric, not merely report a finite answer at one cutoff.

For a continuum local algebra, a bounded SLD operator need not exist even when a regulated quadratic form converges. Restricting the state to a subalgebra cannot increase either monotone metric, but it also does not prove ultraviolet finiteness. The strongest justified statement here is the explicit finite-regulator result plus a separately proved limit under the stated source-domain condition.

Calling one measurement’s Fisher information “the QFI.” The SLD value is an optimization over the allowed measurement class. State that class and whether the local optimum is implementable.

Equating SLD and BKM because a diagonal example agrees. Their Petz normalizations agree on commuting directions; their noncommuting kernels do not. Geometric Bures normalization adds a further factor of 1/41/4.

Removing the cutoff without testing the tangent. A square-summable displacement can have finite SLD QFI but infinite energy and BKM response. Report the cutoff law and the common operator domain.

  1. Let ρλ=diag⁡(p(λ),1−p(λ))\rho_\lambda=\operatorname{diag}(p(\lambda),1-p(\lambda)). Compute the SLD and show that the SLD and BKM metrics coincide.
Solution

The tangent is X=diag⁡(p˙,−p˙)X=\operatorname{diag}(\dot p,-\dot p) and commutes with ρ\rho. Hence L=diag⁡(p˙/p,−p˙/(1−p))L=\operatorname{diag}(\dot p/p,-\dot p/(1-p)), so

FSLD=(p˙)2p+(p˙)21−p=(p˙)2p(1−p).F_{\rm SLD} =\frac{(\dot p)^2}{p}+\frac{(\dot p)^2}{1-p} =\frac{(\dot p)^2}{p(1-p)}.

For diagonal entries the BKM divided difference equals 1/pn1/p_n, giving the same result. The calculation also shows why equality in a classical example says nothing about a noncommuting direction.

  1. Derive the single-mode displacement result FSLD=2g2tanh⁡(x/2)F_{\rm SLD}=2g^2\tanh(x/2) and gBKM=xg2g_{\rm BKM}=xg^2, where x=βωx=\beta\omega.
Solution

Write pn=(1−r)rnp_n=(1-r)r^n with r=e−xr=e^{-x} and use ∣⟨n+1∣p∣n⟩∣2=(n+1)/2\lvert\langle n+1\lvert p\rvert n\rangle\rvert^2=(n+1)/2. Combining the two matrix orientations gives

FSLD=4g2∑n≥0(pn−pn+1)2pn+pn+1n+12.F_{\rm SLD} =4g^2\sum_{n\geq0} \frac{(p_n-p_{n+1})^2}{p_n+p_{n+1}} \frac{n+1}{2}.

Since (pn−pn+1)2/(pn+pn+1)=pn(1−r)2/(1+r)(p_n-p_{n+1})^2/(p_n+p_{n+1})=p_n(1-r)^2/(1+r) and ∑npn(n+1)=1/(1−r)\sum_n p_n(n+1)=1/(1-r),

FSLD=2g21−r1+r=2g2tanh⁡(x/2).F_{\rm SLD}=2g^2\frac{1-r}{1+r}=2g^2\tanh(x/2).

The displacement raises the oscillator energy by ωλ2g2/2\omega\lambda^2g^2/2. Thermal relative entropy is β\beta times that increase, so comparison with S=λ2gBKM/2S=\lambda^2g_{\rm BKM}/2 gives gBKM=xg2g_{\rm BKM}=xg^2.

  1. In ds=3d_s=3, take g(k)∼k−αg(k)\sim k^{-\alpha}. Classify the SLD and BKM ultraviolet behavior for α=3/2\alpha=3/2, 7/47/4, and 22.
Solution

The SLD threshold is 2α>32\alpha>3 and the BKM threshold is 2α>42\alpha>4. At α=3/2\alpha=3/2, SLD diverges logarithmically and BKM diverges as a positive power. At α=7/4\alpha=7/4, SLD converges but BKM still has a power divergence. At α=2\alpha=2, SLD converges while BKM is exactly at its logarithmic threshold. Thus none of the three choices gives a finite BKM continuum metric; one needs α>2\alpha>2.

  • Braunstein, Samuel L., and Carlton M. Caves. “Statistical Distance and the Geometry of Quantum States.” Physical Review Letters 72 (1994): 3439–3443. DOI.
  • Lesniewski, Andrew, and Mary Beth Ruskai. “Monotone Riemannian Metrics and Relative Entropy on Non-Commutative Probability Spaces.” Journal of Mathematical Physics 40 (1999): 5702–5724. DOI; arXiv.
  • Monras, Alex. “Phase Space Formalism for Quantum Estimation of Gaussian States.” arXiv:1303.3682 (2013). arXiv.

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