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Classical and Quantum Fisher Information

Fisher information quantifies how quickly nearby parameter values become statistically distinguishable. In a quantum experiment there are two distinct levels:

  • classical Fisher information FCF_C belongs to the outcome distribution produced by a specified measurement;
  • quantum Fisher information FQF_Q is the greatest classical Fisher information available from the parameterized quantum state when all POVMs on that state are considered.

That distinction is operational. A state may contain information that the implemented detector does not extract. Conversely, a reported FQF_Q does not identify a realizable detector, remove nuisance parameters, resolve global aliases, or guarantee good finite-sample performance.

The following derivation connects the likelihood to the SLD, works through qubit examples, and explains the qualifications at rank changes and in multiparameter estimation.

Required background. Use classical Fisher information for scores and regularity assumptions, POVMs for outcome probabilities, and density operators for spectra and mixtures.

Let a real parameter θ\theta be encoded in a density operator ρθ\rho_\theta. A parameter-independent POVM

M={Mx}x,Mx⪰0,∑xMx=I,\mathsf M=\{M_x\}_x, \qquad M_x\succeq0, \qquad \sum_x M_x=I,

produces the probabilities

p(x∣θ,M)=Tr⁡(ρθMx).p(x\mid\theta,\mathsf M) = \operatorname{Tr}(\rho_\theta M_x).

For discrete outcomes, the classical Fisher information of this measurement is

FC(θ;M)=∑x:px>0(∂θpx)2px,px=Tr⁡(ρθMx).F_C(\theta;\mathsf M) = \sum_{x:p_x>0} \frac{(\partial_\theta p_x)^2}{p_x}, \qquad p_x=\operatorname{Tr}(\rho_\theta M_x).

For a continuous record, replace the sum by an integral with respect to the declared reference measure. Outcomes whose probability vanishes require a limit or a support-sensitive treatment; silently inserting px=0p_x=0 into the fraction is not meaningful.

The notation FC(θ;M)F_C(\theta;\mathsf M) deliberately names the measurement. Changing the basis, detector resolution, acceptance rule, or coarse graining changes the likelihood and can change the available information.

Classical Fisher Information After Measurement

Section titled “Classical Fisher Information After Measurement”

The score of one observed outcome is

sθ(x)=∂θlog⁡p(x∣θ,M).s_\theta(x) = \partial_\theta\log p(x\mid\theta,\mathsf M).

Under the usual regularity assumptions, Eθ[sθ]=0\mathbb E_\theta[s_\theta]=0, and

FC(θ;M)=Eθ[sθ2].F_C(\theta;\mathsf M) = \mathbb E_\theta[s_\theta^2].

Thus FCF_C is a local signal-to-noise ratio for the score. If θ\theta changes the probabilities strongly compared with their statistical fluctuations, FCF_C is large. If all probabilities are positive and locally stationary, FC=0F_C=0 for that measurement even when another measurement would be informative. Zero-probability outcomes require the separate support analysis noted above.

For ν\nu independent repetitions of the same measurement,

FC(ν)=νFC(1).F_C^{(\nu)} = \nu F_C^{(1)}.

This additivity is a statement about independent likelihoods, not about every experiment containing ν\nu nominal shots. Drift, temporal correlations, adaptive settings, dead time, and postselection must be represented in the actual joint likelihood.

Classical postprocessing cannot increase Fisher information. If yy is generated from xx by a parameter-independent stochastic map K(y∣x)K(y\mid x), then

FC(Y;θ)≤FC(X;θ).F_C(Y;\theta) \le F_C(X;\theta).

Discarding time tags, binning a continuous signal too coarsely, thresholding an analog record, or merging detector outcomes may therefore lose sensitivity.

Quantum Fisher Information as an Optimization

Section titled “Quantum Fisher Information as an Optimization”

For a one-parameter state family, the SLD quantum Fisher information is

FQ(θ)=sup⁡MFC(θ;M),F_Q(\theta) = \sup_{\mathsf M} F_C(\theta;\mathsf M),

where the supremum is over parameter-independent POVMs on the system at the specified operating point. In a regular finite-dimensional one-parameter model, this supremum is attained locally by a projective measurement in an eigenbasis of the SLD defined below.

The optimization has three important qualifications:

  1. It is local in θ\theta. It compares infinitesimally neighboring states, not all parameter values across a wide prior interval.
  2. The optimizing measurement can depend on the unknown true value. Practical protocols use prior localization, adaptive measurements, covariant constructions, or a detector that is near-optimal over a declared range.
  3. The optimization must respect the physical measurement class. If only a restricted set A\mathcal A is implementable, the relevant quantity is
FA(θ)=sup⁡M∈AFC(θ;M),F_{\mathcal A}(\theta) = \sup_{\mathsf M\in\mathcal A} F_C(\theta;\mathsf M),

which may be strictly smaller than FQF_Q.

The symmetric logarithmic derivative LθL_\theta is a Hermitian operator satisfying

∂θρθ=12(Lθρθ+ρθLθ).\partial_\theta\rho_\theta = \frac12 \left( L_\theta\rho_\theta + \rho_\theta L_\theta \right).

The corresponding quantum Fisher information is

FQ(θ)=Tr⁡(ρθLθ2)=Tr⁡[(∂θρθ)Lθ].\begin{aligned} F_Q(\theta) &= \operatorname{Tr}(\rho_\theta L_\theta^2)\\ &= \operatorname{Tr} \left[ (\partial_\theta\rho_\theta)L_\theta \right]. \end{aligned}

If ρθ\rho_\theta is not full rank, LθL_\theta need not be unique on the kernel of ρθ\rho_\theta. Its action on the support determines FQF_Q, so this nonuniqueness does not change the value in a regular fixed-rank model. Points where rank or support changes deserve separate care: the SLD expression, its nearby limit, and finite-difference distinguishability need not behave as a naive smooth formula suggests.

The SLD is not usually an observable that the parameter encoding literally couples to. It is the locally optimal score operator for the quantum model.

Why Every Measurement Obeys the Quantum Bound

Section titled “Why Every Measurement Obeys the Quantum Bound”

For a fixed POVM element MxM_x,

∂θpx=Tr⁡[(∂θρθ)Mx]=Re⁡Tr⁡(ρθLθMx).\begin{aligned} \partial_\theta p_x &= \operatorname{Tr} \left[ (\partial_\theta\rho_\theta)M_x \right]\\ &= \operatorname{Re} \operatorname{Tr} (\rho_\theta L_\theta M_x). \end{aligned}

A Hilbert–Schmidt Cauchy–Schwarz inequality gives

(∂θpx)2≤px Tr⁡(ρθLθMxLθ).(\partial_\theta p_x)^2 \le p_x\, \operatorname{Tr} (\rho_\theta L_\theta M_x L_\theta).

Summing over outcomes yields the Braunstein–Caves inequality,

FC(θ;M)≤∑xTr⁡(ρθLθMxLθ)=Tr⁡(ρθLθ2)=FQ(θ).\begin{aligned} F_C(\theta;\mathsf M) &\le \sum_x \operatorname{Tr} (\rho_\theta L_\theta M_x L_\theta)\\ &= \operatorname{Tr}(\rho_\theta L_\theta^2)\\ &= F_Q(\theta). \end{aligned}

At a known operating point, measuring the spectral projectors of LθL_\theta saturates the scalar bound under the regularity conditions. This proves a local optimization statement. It does not prove that one fixed detector is globally optimal or that the resulting estimator reaches a variance bound for a finite data set.

Write the spectral decomposition

ρθ=∑iλi∣i⟩⟨i∣.\rho_\theta = \sum_i \lambda_i \lvert i\rangle\langle i\rvert.

In this instantaneous eigenbasis, the SLD matrix elements on the support are

⟨i∣Lθ∣j⟩=2⟨i∣∂θρθ∣j⟩λi+λj,λi+λj>0.\langle i|L_\theta|j\rangle = \frac{ 2\langle i|\partial_\theta\rho_\theta|j\rangle }{ \lambda_i+\lambda_j }, \qquad \lambda_i+\lambda_j>0.

Therefore

FQ(θ)=2∑i,j:λi+λj>0∣⟨i∣∂θρθ∣j⟩∣2λi+λj.F_Q(\theta) = 2 \sum_{i,j:\lambda_i+\lambda_j>0} \frac{ |\langle i|\partial_\theta\rho_\theta|j\rangle|^2 }{ \lambda_i+\lambda_j }.

Separating eigenvalue and eigenvector changes gives

FQ=∑i:λi>0(∂θλi)2λi+2∑i≠j:λi+λj>0(λi−λj)2λi+λj∣⟨i∣∂θj⟩∣2.F_Q ={} \sum_{i:\lambda_i>0} \frac{(\partial_\theta\lambda_i)^2}{\lambda_i} + 2\sum_{i\ne j:\lambda_i+\lambda_j>0} \frac{(\lambda_i-\lambda_j)^2}{\lambda_i+\lambda_j} |\langle i|\partial_\theta j\rangle|^2.

The first line is information in changing eigenvalues and is classical in the instantaneous eigenbasis. The second is information in rotating eigenvectors, which requires a measurement sensitive to coherence between those directions.

For a commuting family,

[ρθ,ρθ′]=0for all nearby θ,θ′,[\rho_\theta,\rho_{\theta'}]=0 \quad \text{for all nearby }\theta,\theta',

one common eigenbasis measures all the available information, and FQF_Q reduces to the classical Fisher information of the eigenvalues.

For a differentiable normalized state ∣ψθ⟩\lvert\psi_\theta\rangle, write

∣ψ˙θ⟩=∂θ∣ψθ⟩.\lvert\dot\psi_\theta\rangle = \partial_\theta\lvert\psi_\theta\rangle.

The pure-state quantum Fisher information is

FQ[∣ψθ⟩]=4(⟨ψ˙θ∣ψ˙θ⟩−∣⟨ψθ∣ψ˙θ⟩∣2).F_Q[\lvert\psi_\theta\rangle] = 4 \left( \langle\dot\psi_\theta|\dot\psi_\theta\rangle - |\langle\psi_\theta|\dot\psi_\theta\rangle|^2 \right).

The subtraction removes parameter-dependent global phase. If ∣ψθ⟩=eiχ(θ)∣ψ0⟩\lvert\psi_\theta\rangle=e^{i\chi(\theta)}\lvert\psi_0\rangle, the ray does not change and FQ=0F_Q=0.

For a unitary encoding

∣ψθ⟩=e−iθG∣ψ0⟩,\lvert\psi_\theta\rangle = e^{-i\theta G} \lvert\psi_0\rangle,

with a parameter-independent Hermitian generator GG and dimensionless phase θ\theta,

FQ=4Var⁡ψ0(G).F_Q = 4\operatorname{Var}_{\psi_0}(G).

This identity is exact for pure states. For a mixed input under the same unitary encoding,

FQ[ρ,G]=2∑i,j:λi+λj>0(λi−λj)2λi+λj∣⟨i∣G∣j⟩∣2,F_Q[\rho,G] = 2 \sum_{i,j:\lambda_i+\lambda_j>0} \frac{(\lambda_i-\lambda_j)^2}{\lambda_i+\lambda_j} |\langle i|G|j\rangle|^2,

and only the inequality

FQ[ρ,G]≤4Var⁡ρ(G)F_Q[\rho,G] \le 4\operatorname{Var}_\rho(G)

holds in general. A mixed state can have nonzero generator variance entirely from classical uncertainty while commuting with GG; then the state does not move under the encoding and its QFI is zero.

Consider

∣ψθ⟩=∣0⟩+eiθ∣1⟩2.\lvert\psi_\theta\rangle = \frac{ \lvert0\rangle+e^{i\theta}\lvert1\rangle }{\sqrt2}.

Direct substitution into the pure-state formula gives

FQ=1.F_Q=1.

At a provisional operating point θ0\theta_0, measure the observable

Yθ0=−sin⁡θ0 X+cos⁡θ0 Y.Y_{\theta_0} = -\sin\theta_0\,X + \cos\theta_0\,Y.

Its two outcome probabilities are

p±(θ)=12[1±sin⁡(θ−θ0)].p_\pm(\theta) = \frac12 \left[ 1\pm\sin(\theta-\theta_0) \right].

At θ=θ0\theta=\theta_0,

FC(θ0;Yθ0)=1=FQ.F_C(\theta_0;Y_{\theta_0}) = 1 = F_Q.

The detector is locally optimal because it measures the quadrature with the largest slope at the operating point. But the state and likelihood are periodic, so FQ=1F_Q=1 alone cannot identify which 2π2\pi branch contains the true phase. Dynamic range and phase unwrapping belong to the full estimation protocol.

Let

ρθ=θ∣0⟩⟨0∣+(1−θ)∣1⟩⟨1∣,0<θ<1.\rho_\theta = \theta\lvert0\rangle\langle0\rvert + (1-\theta)\lvert1\rangle\langle1\rvert, \qquad 0<\theta<1.

Only the eigenvalues change. Measuring in the computational basis gives a Bernoulli model and

FC=1θ+11−θ=1θ(1−θ).F_C = \frac1\theta+ \frac1{1-\theta} = \frac1{\theta(1-\theta)}.

The spectral QFI formula gives the same result, so

FQ=FC(Z).F_Q = F_C(Z).

No coherent measurement is needed because the model is already classical in a common basis. The divergence near θ=0\theta=0 or 11 is also a warning: boundary points violate some regularity assumptions behind familiar local asymptotic conclusions.

An equatorial qubit with reduced coherence can be written

ρθ=12[I+η(cos⁡θ X+sin⁡θ Y)],0≤η≤1.\rho_\theta = \frac12 \left[ I+ \eta (\cos\theta\,X+\sin\theta\,Y) \right], \qquad 0\le\eta\le1.

Its Bloch vector has constant length η\eta and rotates in the equatorial plane. The qubit formula derived below gives

FQ(θ)=η2.F_Q(\theta)=\eta^2.

If the unknown parameter is a frequency ω\omega, the phase is θ=ωt\theta=\omega t, and Markovian dephasing gives η=e−γt\eta=e^{-\gamma t}, then one interrogation has

FQ(1)(ω;t)=t2e−2γt.F_Q^{(1)}(\omega;t) = t^2e^{-2\gamma t}.

Ignoring dead time, a total duration TT permits about T/tT/t independent interrogations, so

FQtot=Tt e−2γt.F_Q^{\rm tot} = Tt\,e^{-2\gamma t}.

For γ>0\gamma>0 and many repetitions, with TT large compared with the candidate interrogation time, this continuous-time approximation is maximized at t=1/(2γ)t=1/(2\gamma). A finite experiment also imposes t≤Tt\le T and an integer shot count. Longer coherent evolution increases the phase slope but also destroys contrast. The useful optimization variable is therefore not state QFI in isolation, but total information under the declared time and noise model.

Classical Fisher information for fixed X and Y measurements oscillates below the constant quantum Fisher information of a dephased qubit

For fixed contrast η=0.7\eta=0.7, the encoded state has FQ=η2=0.49F_Q=\eta^2=0.49. An XX measurement attains this at θ=π/2,3π/2\theta=\pi/2,3\pi/2; a YY measurement attains it at θ=0,π,2π\theta=0,\pi,2\pi. At the intervening extrema of its own probability curve each detector is locally insensitive. Changing the measurement basis recovers the information; it does not increase the state’s QFI.

For a full-rank qubit

ρθ=12(I+rθ⋅σ),∣rθ∣<1,\rho_\theta = \frac12 \left(I+\mathbf r_\theta\boldsymbol\cdot\boldsymbol\sigma\right), \qquad |\mathbf r_\theta|<1,

write L=aI+b⋅σL=aI+\mathbf b\boldsymbol\cdot\boldsymbol\sigma. Using the Pauli anticommutator in the SLD equation gives

a+b⋅r=0,b+ar=∂θr.a+\mathbf b\boldsymbol\cdot\mathbf r=0, \qquad \mathbf b+a\mathbf r=\partial_\theta\mathbf r.

Thus a=−(r⋅∂θr)/(1−∣r∣2)a=-(\mathbf r\boldsymbol\cdot\partial_\theta\mathbf r)/(1-|\mathbf r|^2) and b=∂θr−ar\mathbf b=\partial_\theta\mathbf r-a\mathbf r. Substitution into Tr⁡(ρL2)\operatorname{Tr}(\rho L^2) gives

FQ=∣∂θr∣2+(r⋅∂θr)21−∣r∣2.F_Q = |\partial_\theta\mathbf r|^2 + \frac{ (\mathbf r\boldsymbol\cdot\partial_\theta\mathbf r)^2 }{ 1-|\mathbf r|^2 }.

The first term measures motion of the Bloch vector. The second records changes in its length, weighted more strongly near the pure-state boundary. For a smooth path that stays pure, ∣r∣=1|\mathbf r|=1 and r⋅∂θr=0\mathbf r\boldsymbol\cdot\partial_\theta\mathbf r=0; taking the appropriate tangent limit gives

FQ=∣∂θr∣2.F_Q=|\partial_\theta\mathbf r|^2.

One should not substitute ∣r∣=1|\mathbf r|=1 directly into the full-rank formula. The apparent 0/00/0 is the coordinate trace of a rank boundary.

Define the squared Uhlmann fidelity by

F(ρ,σ)=[Tr⁡ρ σρ]2\mathcal F(\rho,\sigma) = \left[ \operatorname{Tr} \sqrt{\sqrt\rho\,\sigma\sqrt\rho} \right]^2

and the Bures distance by

DB2(ρ,σ)=2(1−F(ρ,σ)).D_B^2(\rho,\sigma) = 2\left(1-\sqrt{\mathcal F(\rho,\sigma)}\right).

For a smooth family of constant rank in a neighborhood, these conventions give

DB2(ρθ,ρθ+dθ)=14FQ(θ)dθ2+o(dθ2).D_B^2 (\rho_\theta,\rho_{\theta+d\theta}) = \frac14F_Q(\theta)d\theta^2 + o(d\theta^2).

Thus QFI is four times the Bures metric on a regular state manifold. At a rank-changing point the equality can fail: the Bures distance can detect second-order population changes that the SLD at that point misses. Exercise 9 gives an explicit example; see Šafránek (2017).

For pure states, the Bures metric reduces locally to the Fubini–Study metric:

dsFS2=(⟨ψ˙∣ψ˙⟩−∣⟨ψ∣ψ˙⟩∣2)dθ2=14FQdθ2.ds_{\rm FS}^2 = \left( \langle\dot\psi|\dot\psi\rangle - |\langle\psi|\dot\psi\rangle|^2 \right)d\theta^2 = \frac14F_Qd\theta^2.

Fubini–Study Geometry develops this projective geometry. Here the line element measures sensitivity along the encoded family.

These properties explain how changes of coordinates, preparation, and readout affect sensitivity.

If ϕ=g(θ)\phi=g(\theta) is smooth and locally invertible, then

FQ(ϕ)=FQ(θ)(dθdϕ)2.F_Q^{(\phi)} = F_Q^{(\theta)} \left( \frac{d\theta}{d\phi} \right)^2.

QFI has units inverse to the square of the parameter. A numerical value is not meaningful until the parameter coordinate and units are named.

For independently prepared state families,

FQ(ρθ⊗σθ)=FQ(ρθ)+FQ(σθ).F_Q(\rho_\theta\otimes\sigma_\theta) = F_Q(\rho_\theta)+F_Q(\sigma_\theta).

Hence NN independent identical probes carry NFQ(1)NF_Q^{(1)}. This is the information-theoretic origin of the inverse-square-root precision scaling developed on the Standard Quantum Limit page.

For parameter-independent mixing probabilities qkq_k,

FQ(∑kqkρk,θ)≤∑kqkFQ(ρk,θ).F_Q \left( \sum_k q_k\rho_{k,\theta} \right) \le \sum_k q_kF_Q(\rho_{k,\theta}).

Unrecorded classical mixing cannot improve sensitivity. If the weights qk(θ)q_k(\theta) themselves depend on the parameter, they carry classical information and the useful extended bound is

FQ(∑kqk(θ)ρk,θ)≤FC({qk})+∑kqkFQ(ρk,θ).F_Q \left( \sum_k q_k(\theta)\rho_{k,\theta} \right) \le F_C(\{q_k\}) + \sum_k q_kF_Q(\rho_{k,\theta}).

For a parameter-independent quantum channel Λ\Lambda,

FQ[Λ(ρθ)]≤FQ(ρθ).F_Q[\Lambda(\rho_\theta)] \le F_Q(\rho_\theta).

Measurement is such a channel from a quantum state to a classical register, so this monotonicity contains FC≤FQF_C\le F_Q as a special case. Noise after encoding cannot create information about θ\theta if the noise mechanism itself has no parameter dependence.

If a device or measurement depends on θ\theta, its dependence can add a new encoding pathway. It must be included in the physical model; it is not a counterexample to parameter-independent data processing.

Suppose orthogonal flag states preserve which branch occurred:

ρθXQ=∑kqk(θ)∣k⟩⟨k∣⊗ρk,θ.\rho_\theta^{XQ} = \sum_k q_k(\theta) \lvert k\rangle\langle k\rvert \otimes \rho_{k,\theta}.

Then the information decomposes exactly as

FQ(ρθXQ)=FC({qk})+∑kqkFQ(ρk,θ).F_Q(\rho_\theta^{XQ}) = F_C(\{q_k\}) + \sum_k q_kF_Q(\rho_{k,\theta}).

This formula is useful for heralding, erasure flags, and branch-resolved experiments. Throwing away the flag applies a channel and can only reduce the information.

For a locally unbiased scalar estimator based on ν\nu independent copies, the classical and quantum Cramér–Rao inequalities form the chain

Var⁡θ(θ^)≥1νFC(θ;M)≥1νFQ(θ).\operatorname{Var}_\theta(\hat\theta) \ge \frac{1}{\nu F_C(\theta;\mathsf M)} \ge \frac{1}{\nu F_Q(\theta)}.

Each inequality has its own attainability question. The first depends on the estimator, sample size, model regularity, and likelihood. The second depends on the measurement and operating point. Equality in both generally requires a measurement that extracts the QFI and an estimator operating in a regime where the classical bound is attainable.

Cramér–Rao Bounds develops the corresponding assumptions for biased, Bayesian, finite-sample, and multiparameter inference. QFI supplies a precision benchmark; an achieved error bar requires an estimator and data.

For parameters θ=(θ1,…,θm)\boldsymbol\theta=(\theta^1,\ldots,\theta^m), define one SLD for each tangent direction,

∂μρ=12(Lμρ+ρLμ).\partial_\mu\rho = \frac12 (L_\mu\rho+\rho L_\mu).

The SLD quantum Fisher information matrix is

(JQ)μν=12Tr⁡[ρ{Lμ,Lν}]=Re⁡Tr⁡(ρLμLν).\begin{aligned} (J_Q)_{\mu\nu} &= \frac12 \operatorname{Tr} \left[ \rho\{L_\mu,L_\nu\} \right]\\ &= \operatorname{Re} \operatorname{Tr}(\rho L_\mu L_\nu). \end{aligned}

For any real direction u\mathbf u in parameter space,

uTJQu\mathbf u^{\mathsf T}J_Q\mathbf u

is the scalar QFI for motion along that direction. A singular JQJ_Q indicates a direction with no first-order statistical sensitivity. This need not imply local non-identifiability: a probability proportional to θ3\theta^3 plus a positive constant is injective near zero despite its vanishing derivative there.

The formal SLD matrix bound is

Cov⁡(θ^)⪰1νJQ−1,\operatorname{Cov}(\hat{\boldsymbol\theta}) \succeq \frac1\nu J_Q^{-1},

under local-unbiasedness and regularity assumptions. Unlike the scalar case, one measurement need not attain all matrix directions simultaneously. The SLDs can encode incompatible optimal observables.

If Hermitian SLD operators can be chosen to commute, their common eigenbasis provides a sufficient locally optimal measurement. Merely commuting after compression to the occupied subspace is not sufficient: for a pure state that subspace is one-dimensional even when different tangent measurements are incompatible. A weaker mean-commutator condition,

Tr⁡[ρ[Lμ,Lν]]=0,\operatorname{Tr} \left[ \rho[L_\mu,L_\nu] \right] =0,

characterizes equality of the SLD and Holevo bounds in regular finite-dimensional models, with asymptotic attainability under the usual independent-copy and collective-measurement assumptions (Ragy, Jarzyna, and Demkowicz-Dobrzański, 2016). When incompatibility remains, weighted scalar costs and the Holevo Cramér–Rao bound give the operational joint limit; optimizing each diagonal element of JQJ_Q separately overstates what one common experiment can deliver.

Partition the parameter vector into a target α\alpha and nuisance parameters λ\boldsymbol\lambda. Formally partition the QFI matrix as

JQ=(JααJαλJλαJλλ).J_Q = \begin{pmatrix} J_{\alpha\alpha} & J_{\alpha\lambda}\\ J_{\lambda\alpha} & J_{\lambda\lambda} \end{pmatrix}.

When the relevant inverses and attainability assumptions hold, the Schur complement

Jeff=Jαα−JαλJλλ−1JλαJ_{\rm eff} = J_{\alpha\alpha} - J_{\alpha\lambda} J_{\lambda\lambda}^{-1} J_{\lambda\alpha}

is the information remaining about α\alpha when λ\boldsymbol\lambda must also be inferred. It is no larger than JααJ_{\alpha\alpha}. Calibration drift, unknown contrast, loss, phase offsets, and background rates can therefore erase an apparent one-parameter advantage.

For a quantum model this Schur complement is an SLD-based local benchmark. It does not remove multiparameter measurement incompatibility; a complete claim must analyze the attainable cost for the joint model.

Often the unknown parameter belongs to a channel Eθ\mathcal E_\theta, not to a state supplied in advance. A single-use, ancilla-assisted channel QFI can be defined by

FQ(Eθ)=sup⁡ρSAFQ[(Eθ⊗IA)(ρSA)].\mathcal F_Q(\mathcal E_\theta) = \sup_{\rho_{SA}} F_Q \left[ (\mathcal E_\theta\otimes\mathcal I_A)(\rho_{SA}) \right].

The input probe and ancilla are independent of the unknown parameter. The supremum must also state any energy or dimension constraints; without an energy bound it may be infinite for bosonic channels. The optimization includes the probe and any retained ancilla. With many channel uses, parallel entanglement, sequential controls, adaptive operations, and error correction may change the attainable information. The QFI of one chosen output state is therefore not automatically the ultimate limit of the physical sensor.

Noise should be placed inside the channel before optimization. Purification and Kraus-representation methods can upper-bound the output QFI, while channel extension methods expose when an ancilla helps and when asymptotic scaling is limited to linear growth. Quantum Channels and Noise develops the completely positive maps used here.

For NN independent equatorial qubits acquiring the same phase, additivity gives

FQproduct=N.F_Q^{\rm product}=N.

For an ideal NN-qubit GHZ state under the collective generator

Jz=12∑k=1NZk,J_z=\frac12\sum_{k=1}^N Z_k,

the pure-state variance formula gives

FQGHZ=4Var⁡(Jz)=N2.F_Q^{\rm GHZ} = 4\operatorname{Var}(J_z) = N^2.

These equations compare ideal unitary state families. Converting them into an error law requires preparation and readout costs, interrogation time, losses, repetitions, a phase range, and an estimator. Standard Quantum Limit develops the independent-probe benchmark, Heisenberg Scaling treats the ideal quadratic-QFI regime and its limits, and Spin Squeezing connects an implemented collective-spin readout to entanglement criteria.

What Quantum Fisher Information Does Not Tell You

Section titled “What Quantum Fisher Information Does Not Tell You”

QFI answers a sharply defined question:

How distinguishable are infinitesimally neighboring states under the best locally chosen allowed measurement?

It does not answer several other questions without additional analysis:

Question Additional object needed
Which detector should be built? an attainable POVM or receiver model
Which parameter branch is correct? prior range, global likelihood, or adaptive localization
What error occurs after 20 shots? finite-sample estimator distribution or interval construction
Is a multiparameter matrix bound attainable? compatibility and Holevo-bound analysis
Does postselection improve total performance? success/failure likelihood and full resource count
Is the sensor better than a baseline? matched task, resources, noise, and decision metric
Is the model calibrated? validation data and nuisance-parameter treatment

Large QFI is valuable evidence of local quantum sensitivity. It is not a synonym for accuracy, resolution, bandwidth, dynamic range, robustness, or verified quantum advantage.

1. Locally optimal qubit phase measurement

Section titled “1. Locally optimal qubit phase measurement”

For

∣ψθ⟩=∣0⟩+eiθ∣1⟩2,\lvert\psi_\theta\rangle = \frac{\lvert0\rangle+e^{i\theta}\lvert1\rangle}{\sqrt2},

compute FQF_Q and show that measuring Yθ0Y_{\theta_0} at θ=θ0\theta=\theta_0 attains it.

Solution

The derivative is

∣ψ˙θ⟩=ieiθ∣1⟩2.\lvert\dot\psi_\theta\rangle = \frac{i e^{i\theta}\lvert1\rangle}{\sqrt2}.

Hence

⟨ψ˙∣ψ˙⟩=12,∣⟨ψ∣ψ˙⟩∣2=14,\langle\dot\psi|\dot\psi\rangle=\frac12, \qquad |\langle\psi|\dot\psi\rangle|^2=\frac14,

and

FQ=4(12−14)=1.F_Q=4\left(\frac12-\frac14\right)=1.

For Yθ0Y_{\theta_0},

p±=12[1±sin⁡(θ−θ0)].p_\pm = \frac12[1\pm\sin(\theta-\theta_0)].

At θ0\theta_0, p±=1/2p_\pm=1/2 and ∂θp±=±1/2\partial_\theta p_\pm=\pm1/2. Therefore

FC=(1/2)21/2+(−1/2)21/2=1=FQ.F_C = \frac{(1/2)^2}{1/2} + \frac{(-1/2)^2}{1/2} =1=F_Q.

For

ρθ=θ∣0⟩⟨0∣+(1−θ)∣1⟩⟨1∣,\rho_\theta = \theta\lvert0\rangle\langle0\rvert + (1-\theta)\lvert1\rangle\langle1\rvert,

find the SLD and verify FQ=1/[θ(1−θ)]F_Q=1/[\theta(1-\theta)].

Solution

Because ρθ\rho_\theta and its derivative are diagonal, the SLD is diagonal:

Lθ=1θ∣0⟩⟨0∣−11−θ∣1⟩⟨1∣.L_\theta = \frac1\theta\lvert0\rangle\langle0\rvert - \frac1{1-\theta}\lvert1\rangle\langle1\rvert.

Indeed,

12(Lρ+ρL)=∣0⟩⟨0∣−∣1⟩⟨1∣=∂θρ.\frac12(L\rho+\rho L) = \lvert0\rangle\langle0\rvert - \lvert1\rangle\langle1\rvert = \partial_\theta\rho.

Then

FQ=Tr⁡(ρL2)=1θ+11−θ=1θ(1−θ).F_Q = \operatorname{Tr}(\rho L^2) = \frac1\theta+ \frac1{1-\theta} = \frac1{\theta(1-\theta)}.

Computational-basis measurement produces the same Bernoulli Fisher information and is optimal.

3. Generator variance can overestimate mixed-state sensitivity

Section titled “3. Generator variance can overestimate mixed-state sensitivity”

Let

ρ=12(∣0⟩⟨0∣+∣1⟩⟨1∣)\rho = \frac12 (\lvert0\rangle\langle0\rvert+ \lvert1\rangle\langle1\rvert)

and G=Z/2G=Z/2. Compare 4Var⁡ρ(G)4\operatorname{Var}_\rho(G) with the QFI of e−iθGρeiθGe^{-i\theta G}\rho e^{i\theta G}.

Solution

The state is I/2I/2, so it commutes with every generator and

e−iθGρeiθG=ρ.e^{-i\theta G}\rho e^{i\theta G}=\rho.

Therefore ∂θρθ=0\partial_\theta\rho_\theta=0 and FQ=0F_Q=0. But

⟨G⟩=0,⟨G2⟩=14,\langle G\rangle=0, \qquad \langle G^2\rangle=\frac14,

so

4Var⁡ρ(G)=1.4\operatorname{Var}_\rho(G)=1.

The variance reflects classical uncertainty over generator eigenvalues, not coherent motion of the mixed state. This is why FQ=4Var⁡(G)F_Q=4\operatorname{Var}(G) cannot be extended from pure states as an equality.

4. Optimize a dephasing-limited interrogation

Section titled “4. Optimize a dephasing-limited interrogation”

Suppose one frequency interrogation has

FQ(1)(ω;t)=t2e−2γtF_Q^{(1)}(\omega;t)=t^2e^{-2\gamma t}

and γ>0\gamma>0. Neglect dead time and assume T≫1/γT\gg1/\gamma, so the continuous approximation T/tT/t describes many independent shots. Find the optimal tt and total QFI.

Solution

The total information is

FQtot(t)=Ttt2e−2γt=Tte−2γt.F_Q^{\rm tot}(t) = \frac{T}{t}t^2e^{-2\gamma t} = Tt e^{-2\gamma t}.

Differentiating gives

dFQtotdt=Te−2γt(1−2γt).\frac{dF_Q^{\rm tot}}{dt} = T e^{-2\gamma t}(1-2\gamma t).

Thus

t⋆=12γt_\star=\frac1{2\gamma}

and

FQtot(t⋆)=T2γe.F_Q^{\rm tot}(t_\star) = \frac{T}{2\gamma e}.

Any preparation or readout dead time changes the repetition count and shifts this optimum.

A parameter-independent erasure occurs with probability qq. Successful outputs retain ρθ\rho_\theta, while erased outputs become an orthogonal flag ∣e⟩\lvert e\rangle. Show that

FQout=(1−q)FQ(ρθ).F_Q^{\rm out}=(1-q)F_Q(\rho_\theta).
Solution

The output is a flagged direct sum,

ρθout=(1−q)ρθ⊕q∣e⟩⟨e∣.\rho_\theta^{\rm out} = (1-q)\rho_\theta \oplus q\lvert e\rangle\langle e\rvert.

The weights are independent of θ\theta, so their classical Fisher information is zero. The erasure branch is also independent of θ\theta. The flagged-state decomposition therefore gives

FQout=0+(1−q)FQ(ρθ)+qFQ(∣e⟩)=(1−q)FQ(ρθ).\begin{aligned} F_Q^{\rm out} &= 0+(1-q)F_Q(\rho_\theta) +qF_Q(\lvert e\rangle)\\ &= (1-q)F_Q(\rho_\theta). \end{aligned}

Quoting QFI only per successful event would omit the resource cost of erased trials.

6. Parameter-dependent heralding probabilities

Section titled “6. Parameter-dependent heralding probabilities”

Consider a flagged state

ρθXQ=q(θ)∣s⟩⟨s∣⊗ρθ+[1−q(θ)]∣f⟩⟨f∣⊗τ,\rho_\theta^{XQ} = q(\theta)\lvert s\rangle\langle s\rvert\otimes\rho_\theta + [1-q(\theta)]\lvert f\rangle\langle f\rvert\otimes\tau,

where τ\tau is parameter independent. Compute its QFI.

Solution

The orthogonal flag preserves both branch probabilities, so the exact decomposition applies:

FQ=FC({q,1−q})+qFQ(ρθ)+(1−q)FQ(τ).F_Q = F_C(\{q,1-q\}) + qF_Q(\rho_\theta) + (1-q)F_Q(\tau).

Since FQ(τ)=0F_Q(\tau)=0 and a Bernoulli distribution has Fisher information

FC({q,1−q})=[∂θq(θ)]2q(θ)[1−q(θ)],F_C(\{q,1-q\}) = \frac{[\partial_\theta q(\theta)]^2}{q(\theta)[1-q(\theta)]},

the result is

FQ=(∂θq)2q(1−q)+qFQ(ρθ).F_Q = \frac{(\partial_\theta q)^2}{q(1-q)} + qF_Q(\rho_\theta).

The success rate is itself data. Conditioning only on successes discards its information and can distort resource comparisons.

For

∣ψ(ϑ,φ)⟩=cos⁡ϑ2∣0⟩+eiφsin⁡ϑ2∣1⟩,\lvert\psi(\vartheta,\varphi)\rangle = \cos\frac\vartheta2\lvert0\rangle + e^{i\varphi}\sin\frac\vartheta2\lvert1\rangle,

show that

JQ=(100sin⁡2ϑ),J_Q = \begin{pmatrix} 1 & 0\\ 0 & \sin^2\vartheta \end{pmatrix},

and diagnose joint attainability away from the poles.

Solution

For pure states, the QFI matrix is four times the real part of the quantum geometric tensor,

(JQ)μν=4Re⁡[⟨∂μψ∣∂νψ⟩−⟨∂μψ∣ψ⟩⟨ψ∣∂νψ⟩].(J_Q)_{\mu\nu} = 4\operatorname{Re} \left[ \langle\partial_\mu\psi|\partial_\nu\psi\rangle - \langle\partial_\mu\psi|\psi\rangle \langle\psi|\partial_\nu\psi\rangle \right].

Direct differentiation gives

(JQ)ϑϑ=1,(JQ)φφ=sin⁡2ϑ,(JQ)ϑφ=0.(J_Q)_{\vartheta\vartheta}=1, \qquad (J_Q)_{\varphi\varphi}=\sin^2\vartheta, \qquad (J_Q)_{\vartheta\varphi}=0.

The imaginary part of the off-diagonal quantum geometric tensor is

Im⁡Qϑφ=14sin⁡ϑ.\operatorname{Im}Q_{\vartheta\varphi} = \frac14\sin\vartheta.

It is nonzero away from the poles, signaling incompatible tangent directions: the measurements separately optimal for polar and azimuthal displacement cannot generally saturate both scalar SLD bounds on one copy. At the poles, φ\varphi is unidentifiable and the matrix is singular.

8. Local information versus global ambiguity

Section titled “8. Local information versus global ambiguity”

An XX measurement on the equatorial phase state gives

p+(θ)=1+cos⁡θ2,p−(θ)=1−cos⁡θ2.p_+(\theta)=\frac{1+\cos\theta}{2}, \qquad p_-(\theta)=\frac{1-\cos\theta}{2}.

Show that its Fisher information is locally one away from zero-probability points, but explain why the measurement cannot distinguish θ\theta from −θ-\theta globally.

Solution

The derivatives are

∂θp+=−12sin⁡θ,∂θp−=12sin⁡θ.\partial_\theta p_+=-\frac12\sin\theta, \qquad \partial_\theta p_-=\frac12\sin\theta.

Therefore

FC=sin⁡2θ/4(1+cos⁡θ)/2+sin⁡2θ/4(1−cos⁡θ)/2=1,\begin{aligned} F_C &= \frac{\sin^2\theta/4}{(1+\cos\theta)/2} + \frac{\sin^2\theta/4}{(1-\cos\theta)/2}\\ &=1, \end{aligned}

The limit is also one as θ→0\theta\to0, but the score information defined by the positive-probability outcomes exactly at zero is zero. These are different quantities at this nonregular point; a limit does not restore the ordinary regular Cramér–Rao assumptions. However,

p±(θ)=p±(−θ),p_\pm(\theta)=p_\pm(-\theta),

so the entire likelihood is invariant under sign reversal. The Fisher information correctly describes local curvature on either branch, but it does not encode the global two-fold ambiguity. A restricted prior, another measurement quadrature, or an adaptive protocol is needed.

Let ρθ=diag⁡(1−θ2,θ2)\rho_\theta=\operatorname{diag}(1-\theta^2,\theta^2) for ∣θ∣<1|\theta|<1. Compare the SLD QFI at zero, its nearby limit, and the Bures distance from ρ0\rho_0.

Solution

At zero, ∂θρ=0\partial_\theta\rho=0, so the SLD formula gives FQ(0)=0F_Q(0)=0. For θ≠0\theta\ne0,

FQ(θ)=4θ21−θ2+4θ2θ2=41−θ2⟶4.F_Q(\theta)=\frac{4\theta^2}{1-\theta^2}+\frac{4\theta^2}{\theta^2} =\frac4{1-\theta^2}\longrightarrow4.

Since the squared fidelity with ρ0\rho_0 is 1−θ21-\theta^2,

DB2(ρ0,ρθ)=2(1−1−θ2)=θ2+O(θ4).D_B^2(\rho_0,\rho_\theta)=2(1-\sqrt{1-\theta^2}) =\theta^2+O(\theta^4).

The Bures coefficient is one, whereas FQ(0)/4=0F_Q(0)/4=0. Rank changes invalidate the fixed-rank identity at that point. The sign of θ\theta also remains globally ambiguous.

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