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Distributed Quantum Sensing

Distributed quantum sensing uses quantum states or quantum correlations shared among spatially separated sensor nodes to estimate a declared property of a field, signal, or set of local parameters. A network might estimate the average phase across several optical paths, a frequency difference between remote clocks, a magnetic-field gradient, or one spatial mode of a fluctuating field. The target is often a weighted functional

q:=wTθ=∑m=1Mwmθm,q := \mathbf w^{\mathsf T}\boldsymbol\theta = \sum_{m=1}^{M}w_m\theta_m,

where θm\theta_m is the response accumulated at node mm and w\mathbf w defines the spatial mode of interest.

The phrase does not mean merely operating several quantum sensors. Independent quantum sensors followed by classical averaging already form a distributed sensor system. A specifically distributed quantum advantage requires a matched comparison showing that inter-node quantum resources improve the declared network task beyond the best allowed node-separable protocol. The comparison must include local nonclassical resources when those are allowed, not only coherent states or independent particles.

Entanglement is strongly task-dependent. It can directly concentrate information into a global functional such as an average. It need not improve, and can even obstruct, reconstruction of every local parameter. Loss at one node can erase a global correlation, and a shared oscillator, synchronized control, accepted-shot rule, or high-power local oscillator may dominate the real resource ledger. The right question is therefore not whether a network is entangled, but whether its complete estimator gains information about the specified spacetime mode per matched resource and per unit wall time.

Quantum Network Architectures owns entanglement services, physical and logical topologies, routing, scheduling, memories, reference-frame metadata, and network control planes. Network Verification owns source and device trust, test-versus-use sampling, topology tests, and service certification. Those topics are used here rather than rebuilt as a network stack.

Classical and Quantum Fisher Information owns Fisher matrices, symmetric logarithmic derivatives, multiparameter compatibility, and attainability. Standard Quantum Limit and Heisenberg Scaling own the general independent-probe and ideal collective scaling laws. GHZ States, Squeezing, and Spin Squeezing own the underlying state families and their local metrological properties.

This page owns the synthesis specific to sensing across nodes:

  • the distinction between estimating a field map and estimating one global field functional;
  • the local-encoding model and network identifiability conditions;
  • matched product-probe, node-separable, and inter-node-entangled benchmarks;
  • discrete-variable and continuous-variable distributed protocols;
  • covariance-mode engineering and rejection of structured nuisance fields;
  • link loss, state age, timing, reference frames, acceptance, and wall-time information rate; and
  • the evidence required to claim a distributed quantum advantage.

Complete clock, magnetometer, inertial-sensor, and optical-interferometer hardware remains in the corresponding platform pages. The focus here is the network estimation problem that begins after local couplings have been specified.

Local responses are filtered field samples

Section titled “Local responses are filtered field samples”

A sensor does not read an instantaneous field value at a mathematical point. Let s(x,t)s(\mathbf x,t) be a physical field and let node mm have position xm\mathbf x_m, calibrated temporal response hm(t)h_m(t), and coupling coefficient κm\kappa_m. Its dimensionless encoded parameter can be written

θm:=κm∫−∞∞hm(t)s(xm,t) dt.\theta_m := \kappa_m \int_{-\infty}^{\infty} h_m(t) s(\mathbf x_m,t) \,\mathrm dt.

Finite sensor volume can be included by replacing the point sample with a spatial integral. Clock interrogation windows, interferometer sensitivity functions, dynamical-decoupling filters, and optical transit times all enter through hmh_m. A network therefore samples a collection of spacetime modes, not an abstract vector detached from hardware.

The target might be:

  • a normalized average, q=M−1∑mθmq=M^{-1}\sum_m\theta_m;
  • a difference, q=(θ1−θ2)/2q=(\theta_1-\theta_2)/2;
  • a finite-difference gradient or curvature;
  • a matched filter for a predicted spatial profile;
  • one coefficient in a basis expansion of a field; or
  • the full vector θ\boldsymbol\theta.

These are different statistical problems. A state optimized for the average may deliberately contain little information about differences. It cannot then be credited with high-resolution imaging of all nodes.

For MM nodes with locally acting generators GmG_m, a standard phase model is

Uθ=⨂m=1Mexp⁡ ⁣(−iθmGm).U_{\boldsymbol\theta} = \bigotimes_{m=1}^{M} \exp\!\left(-i\theta_mG_m\right).

Operators at distinct nodes commute because they act on distinct tensor factors. The input state need not factorize: it may contain particle entanglement within each node, mode entanglement among nodes, or both. After the local interactions, measurements may be local with classical post-processing or genuinely joint. Which operations are allowed is part of the comparison.

For a parameter vector, a measurement produces a Fisher matrix Fθ\mathbf F_{\theta}. If all components are locally identifiable and an unbiased estimator is used in the regular asymptotic regime, then estimating q=wTθq=\mathbf w^{\mathsf T}\boldsymbol\theta through the vector model gives

Var⁡(q^)≥1νwTFθ−1w,\operatorname{Var}(\widehat q) \geq \frac{1}{\nu} \mathbf w^{\mathsf T} \mathbf F_{\theta}^{-1} \mathbf w,

for ν\nu independent repetitions. A generalized inverse and explicit identifiability constraints are required when Fθ\mathbf F_{\theta} is singular.

This expression should not be confused with wTFθw\mathbf w^{\mathsf T}\mathbf F_{\theta}\mathbf w. If the physics instead contains only one unknown qq through θ=vq\boldsymbol\theta=\mathbf vq, then

Fq=vTFθv.F_q = \mathbf v^{\mathsf T} \mathbf F_{\theta} \mathbf v.

The first problem treats orthogonal field modes as unknown nuisance parameters. The second assumes they are absent or known. Switching between them can change a claimed quantum advantage.

Before comparing protocols, state at least:

ItemRequired declaration
estimandfull local vector, weighted functional, field-model coefficient, or detection decision
local responsepositions, coupling gains, generators, temporal filters, and sign conventions
nuisance modelunknown offsets, gradients, oscillator phase, link phase, drift, and environmental modes
quantum boundaryproduct particles, local entanglement, inter-node entanglement, memories, and reference modes allowed
resource boundaryparticles or photons launched, interacting, surviving, and detected; source and link attempts
timingsimultaneous window, allowed latency, cycle time, dead time, and state age
measurementlocal or joint POVM, classical communication, accepted outcomes, and estimator
objectivelocal variance, Bayesian risk, hypothesis error, Fisher information rate, or time to target
validationcalibration data, matched comparator, independent checks, and uncertainty statement

Without this contract, phrases such as “network SQL” or “Heisenberg scaling with node number” are underdetermined. Adding nodes can add probes, spatial coverage, source brightness, reference beams, or interrogation time. Those are different resources.

Task modes, network quantum resources, and the end-to-end resource ledger for distributed quantum sensing

Distributed sensing begins by selecting a weighted spatial mode q=wTθq=\mathbf w^{\mathsf T}\boldsymbol\theta. Product probes, node-local entanglement, and inter-node entanglement have different matched benchmarks. Any gain must survive state distribution, local encoding, readout, accepted outcomes, and cycle-time accounting.

Suppose calibrated local readouts obey

y=θ+ε,E[ε]=0,\mathbf y = \boldsymbol\theta + \boldsymbol\varepsilon, \qquad \mathbb E[\boldsymbol\varepsilon] = \mathbf0,

with noise covariance Σ\boldsymbol\Sigma. The linear estimator q^=wTy\widehat q=\mathbf w^{\mathsf T}\mathbf y has

Var⁡(q^)=wTΣw.\operatorname{Var}(\widehat q) = \mathbf w^{\mathsf T} \boldsymbol\Sigma \mathbf w.

Distributed quantum resources are useful when they reduce this quadratic form for the target mode. Negative cross-covariances can quiet an average; positive cross-covariances can quiet a difference. A covariance ellipse squeezed along one direction must generally broaden along another, so the target weights must be chosen before the state is optimized.

The same formula also describes classical correlations. Synchronous interrogation with a common oscillator can reject oscillator noise in a difference, and subtracting a shared auxiliary sensor can create correlated residuals. Observing wTΣw\mathbf w^{\mathsf T}\boldsymbol\Sigma\mathbf w below the sum of individual variances is therefore not an entanglement witness. A quantum claim needs a state or channel certificate and a bound satisfied by every allowed node-separable protocol.

Suppose local phases follow a known linear field model

θ=Aβ,\boldsymbol\theta = \mathbf A\boldsymbol\beta,

where columns of A\mathbf A contain sampled spatial profiles and β\boldsymbol\beta contains their unknown amplitudes. To estimate coefficient βs\beta_s without bias, weights must satisfy

ATw=es.\mathbf A^{\mathsf T}\mathbf w = \mathbf e_s.

Among linear unbiased estimators, the minimum-variance weights are

w⋆=Σ−1A(ATΣ−1A)−1es,\mathbf w_\star = \boldsymbol\Sigma^{-1}\mathbf A \left( \mathbf A^{\mathsf T} \boldsymbol\Sigma^{-1} \mathbf A \right)^{-1} \mathbf e_s,

provided the indicated matrices have the required rank. Quantum correlations can reshape Σ\boldsymbol\Sigma, but they cannot recover a field component that the sampled response matrix does not identify. Geometry and calibration come before squeezing.

The cleanest hierarchy appears in a normalized qubit-phase model. Assume:

  • NN two-level probes are distributed among MM nodes;
  • each probe samples its local phase once through a generator with eigenvalue span one;
  • all local phases not fixed by the estimand may be unknown;
  • control, contrast, detection, and prior knowledge are ideal; and
  • the experiment is repeated independently ν\nu times.

These assumptions define an illustrative bound, not a universal law for every sensor network.

Let node mm receive nmn_m independent probes, with ∑mnm=N\sum_m n_m=N. Its local Fisher information is at most nmn_m in this normalization. Independent local estimates give

Var⁡(q^)≥1ν∑m=1Mwm2nm.\operatorname{Var}(\widehat q) \geq \frac{1}{\nu} \sum_{m=1}^{M} \frac{w_m^2}{n_m}.

Optimizing the allocation under the fixed total yields

nm=N∣wm∣∥w∥1,Var⁡(q^)prod≥∥w∥12νN,n_m = N \frac{|w_m|}{\|\mathbf w\|_1}, \qquad \operatorname{Var}(\widehat q)_{\rm prod} \geq \frac{\|\mathbf w\|_1^2}{\nu N},

where

∥w∥1:=∑m∣wm∣.\|\mathbf w\|_1 := \sum_m|w_m|.

Equal allocation is optimal only for equal-magnitude weights. Sending the same number of probes to a nearly irrelevant node wastes the declared resource.

Node-separable states with local entanglement

Section titled “Node-separable states with local entanglement”

A stronger comparator allows arbitrary entanglement among the nmn_m probes inside each node but no entanglement between nodes. An ideal local GHZ-like state can provide Fisher information nm2n_m^2 for θm\theta_m, giving

Var⁡(q^)≥1ν∑m=1Mwm2nm2.\operatorname{Var}(\widehat q) \geq \frac{1}{\nu} \sum_{m=1}^{M} \frac{w_m^2}{n_m^2}.

The optimized allocation is now

nm=N∣wm∣2/3∑j∣wj∣2/3,n_m = N \frac{|w_m|^{2/3}}{ \sum_j|w_j|^{2/3} },

and therefore

Var⁡(q^)node-sep≥(∑m∣wm∣2/3)3νN2.\operatorname{Var}(\widehat q)_{\rm node\text{-}sep} \geq \frac{ \left( \sum_m|w_m|^{2/3} \right)^3 }{ \nu N^2 }.

This is the appropriate ideal benchmark when each node may prepare its own nonclassical ensemble. Beating the product-probe SQL while remaining above this bound demonstrates quantum enhancement, but not an advantage due specifically to entanglement between nodes.

A signed GHZ-type state can place the entire weighted functional into one collective phase. Allocate

nm=N∣wm∣∥w∥1n_m = N \frac{|w_m|}{\|\mathbf w\|_1}

and reverse the local coupling for negative wmw_m. The relative phase between the two GHZ branches is

Φ=∑msgn⁡(wm)nmθm=N∥w∥1q.\Phi = \sum_m \operatorname{sgn}(w_m)n_m\theta_m = \frac{N}{\|\mathbf w\|_1} q.

An ideal parity measurement then gives

Var⁡(q^)global≥∥w∥12νN2.\operatorname{Var}(\widehat q)_{\rm global} \geq \frac{\|\mathbf w\|_1^2}{\nu N^2}.

For arbitrary real weights, finite NN may require rounded allocations or a sequence of settings whose average realizes the desired coefficients. The bound also assumes local controls can implement the required signs and that orthogonal field modes are allowed to remain unestimated.

For an equal average, wm=1/Mw_m=1/M, the hierarchy becomes

Var⁡(q^)prod≥1νN,Var⁡(q^)node-sep≥MνN2,Var⁡(q^)global≥1νN2.\begin{aligned} \operatorname{Var}(\widehat q)_{\rm prod} &\geq \frac{1}{\nu N}, \\ \operatorname{Var}(\widehat q)_{\rm node\text{-}sep} &\geq \frac{M}{\nu N^2}, \\ \operatorname{Var}(\widehat q)_{\rm global} &\geq \frac{1}{\nu N^2}. \end{aligned}

The factor MM between the last two variances is the ideal advantage of inter-node entanglement over separately entangled nodes for this particular global task. It is not a generic advantage for estimating all MM phases.

A defensible comparison uses the same:

  • field functional and nuisance model;
  • number of probes that actually sample each location;
  • interrogation time and number of field interactions;
  • source attempts, state-preparation success, and accepted-shot rule;
  • local oscillator, reference beams, ancillas, and memories;
  • loss, detector capability, and classical communication;
  • cycle time and total observation time; and
  • prior range, branch-resolution strategy, and estimator.

A network may have a practical source-count advantage even without a better probe-count bound. For example, splitting one squeezed optical mode among nodes can replace MM independent squeezers. That is valuable engineering, but it should be reported separately from precision scaling at fixed photons incident on the samples.

For commuting local generators and a cost that asks for all local parameters, inter-node entanglement has no generic precision advantage. Broad classes of network problems admit optimal sensor-separable states and local measurements. For noncommuting generators, any intrinsic network advantage is still constrained by multiparameter incompatibility and can be modest.

The situation changes when only one global function is required. A GHZ or collective squeezed mode can spend nearly all available sensitivity on q=wTθq=\mathbf w^{\mathsf T}\boldsymbol\theta while discarding information about orthogonal combinations. That concentration is precisely why it can beat a strategy that separately learns every θm\theta_m before combining them.

This yields a useful design rule:

Entangle across nodes only after deciding which spatial mode may be sacrificed and which one must be measured.

If the application later asks for a different weighting, the state, distribution network, local controls, or measurement basis may need to be reconfigured. One scalar network output cannot be retrospectively promoted to a complete field image.

For qubit or effective-spin nodes, the ideal global protocol prepares a coherence between two many-body branches. Local basis flips can reverse the sign with which selected probes accumulate phase. After encoding, the state has the form

∣ψ(q)⟩=12(∣0⟩+e−iKqq∣1⟩),Kq=N∥w∥1.|\psi(q)\rangle = \frac{1}{\sqrt2} \left( |\mathbf0\rangle + e^{-iK_qq} |\mathbf1\rangle \right), \qquad K_q = \frac{N}{\|\mathbf w\|_1}.

The strings ∣0⟩|\mathbf0\rangle and ∣1⟩|\mathbf1\rangle summarize the two signed branches; they need not be all-zero and all-one strings in the laboratory basis. An analysis rotation followed by local binary measurements produces a parity likelihood

p(π∣q)=12[1+πCcos⁡(Kqq+ϕ0)],π∈{−1,+1},p(\pi\mid q) = \frac12 \left[ 1 + \pi C \cos(K_qq+\phi_0) \right], \qquad \pi\in\{-1,+1\},

where CC is the final network contrast and ϕ0\phi_0 is a controlled analysis phase. The classical Fisher information is

Fq=C2Kq2sin⁡2(Kqq+ϕ0)1−C2cos⁡2(Kqq+ϕ0).F_q = \frac{ C^2K_q^2 \sin^2(K_qq+\phi_0) }{ 1-C^2 \cos^2(K_qq+\phi_0) }.

At a quadrature working point,

Fq=C2Kq2.F_q = C^2K_q^2.

Reduced projection noise alone is not enough: contrast determines the signal slope. A protocol with a narrow parity distribution and nearly vanishing contrast carries little phase information.

The parity can be assembled from local measurement records after classical communication. The sensor qubits need not be physically reunited after encoding. This does not enable faster-than-light signaling: no node can infer the global parity or the distant parameter from its local record alone.

The same factor KqK_q that increases local slope also shortens the fringe period:

q∼q+2πKq.q \sim q + \frac{2\pi}{K_q}.

An ideal NN-probe global state therefore has a local uncertainty of order 1/N1/N but an unambiguous interval of the same order. A broad prior requires a coarse product-state estimate, several interrogation strengths, adaptive analysis phases, or a Bayesian protocol that retains all branches. Quoting the local Fisher information while assuming the correct fringe index is known does not establish globally accurate sensing.

Atomic protocols can create correlations in one ensemble and then divide the atoms into spatial modes. Let Jz,mJ_{z,m} be a local population-difference readout and let

Γmn:=12⟨ΔJz,mΔJz,n+ΔJz,nΔJz,m⟩.\Gamma_{mn} := \frac12 \left\langle \Delta J_{z,m}\Delta J_{z,n} + \Delta J_{z,n}\Delta J_{z,m} \right\rangle.

For a calibrated linear response vector rq\mathbf r_q, an estimator using coefficients a\mathbf a obeys

Δq2=aTΓa∣aTrq∣2.\Delta q^2 = \frac{ \mathbf a^{\mathsf T} \boldsymbol\Gamma \mathbf a }{ |\mathbf a^{\mathsf T}\mathbf r_q|^2 }.

Mode entanglement appears through the off-diagonal blocks of Γ\boldsymbol\Gamma. It is useful only when the quiet covariance direction is aligned with the desired average or difference and the full response slope is retained. Particle entanglement within the original ensemble and mode entanglement among the separated outputs are related but distinct statements.

A network claim must compare the split state with independently optimized local squeezed ensembles when those are physically allowed. Comparing only with coherent-spin states establishes sub-projection-noise operation, not necessarily an inter-node advantage.

Optical and microwave networks often encode weak signals as quadrature displacements or small phase rotations. Choose normalized real mode coefficients umu_m with ∑mum2=1\sum_m u_m^2=1 and define

Xu:=∑m=1MumXm.X_{\mathbf u} := \sum_{m=1}^{M}u_mX_m.

A passive splitter network can distribute one squeezed input so that this collective output quadrature inherits the squeezing:

Var⁡(Xu)=12e−2r\operatorname{Var}(X_{\mathbf u}) = \frac12e^{-2r}

in the convention where vacuum variance is 1/21/2. Orthogonal combinations of the node quadratures contain vacuum noise. Thus each local marginal can look only weakly squeezed while the correctly weighted sum recovers the quiet input mode.

Suppose local transducers produce

E[Xm]=gmθm.\mathbb E[X_m] = g_m\theta_m.

The homodyne weights and splitter amplitudes must be chosen so that the collective response is proportional to q=∑mwmθmq=\sum_mw_m\theta_m. Unequal transducer gains, link attenuation, or local oscillator phases rotate the realized mode away from w\mathbf w. Calibration must therefore determine the response vector, not merely the optical splitting ratios.

A coherent-state network supplies the familiar shot-noise baseline, but it is not always the strongest separable comparator. If local squeezers are allowed, each node can receive its own optimized squeezed state. The comparison must then fix:

  • photons incident on each sample or transducer;
  • coherent displacement and squeezed-vacuum photons;
  • source-to-sample transmission;
  • local-oscillator and reference power when operationally relevant;
  • detector efficiency and bandwidth; and
  • the number and quality of nonclassical sources.

Distributing one squeezed source can outperform MM separable squeezed inputs at fixed total source photons, or it can offer similar sensitivity with fewer squeezers. Those are legitimate but different resource statements. A result should say whether the gain is per sample photon, per generated nonclassical photon, per source, or per wall-clock second.

Spatially correlated noise need not have the same profile as the signal. This creates an opportunity beyond simply reducing white projection noise. Let the Hamiltonian during interrogation be

H=βs∑msmGm+∑μ=1Kβμ∑mnμmGm,H = \beta_s \sum_m s_mG_m + \sum_{\mu=1}^{K} \beta_\mu \sum_m n_{\mu m}G_m,

where s\mathbf s is the sampled signal profile and the vectors nμ\mathbf n_\mu are nuisance profiles. A coherence whose two branches differ by generator vector k\mathbf k accumulates relative phase

Φ=t[βskTs+∑μ=1KβμkTnμ].\Phi = t \left[ \beta_s\mathbf k^{\mathsf T}\mathbf s + \sum_{\mu=1}^{K} \beta_\mu \mathbf k^{\mathsf T}\mathbf n_\mu \right].

If

kTnμ=0for every μ,kTs≠0,\mathbf k^{\mathsf T}\mathbf n_\mu = 0 \quad \text{for every }\mu, \qquad \mathbf k^{\mathsf T}\mathbf s \ne 0,

then the encoded coherence lies in a decoherence-free mode for those nuisance fields while retaining signal response. Multilevel sensors can supply a richer set of branch differences k\mathbf k than two-level sensors.

This protection is model-based. It fails when the nuisance profile is misspecified, node positions drift, coupling gains change, or unmodeled noise has a component along k\mathbf k. A serious experiment measures the residual transfer from every rejected mode and propagates profile uncertainty into the final estimate.

A global GHZ coherence is fragile because every participating subsystem is part of the signal-bearing off-diagonal term. If probe jj survives with probability ηj\eta_j and any loss causes rejection, then

psurv=∏j=1Nηj.p_{\rm surv} = \prod_{j=1}^{N}\eta_j.

If each probe also retains coherence amplitude cjc_j, the final contrast is bounded schematically by

Cnet≲C0∏j=1Ncj.C_{\rm net} \lesssim C_0 \prod_{j=1}^{N}c_j.

The conditional Fisher information may still scale as Cnet2N2C_{\rm net}^2N^2, but the unconditional information per attempt is reduced by survival and preparation probability. Independent probes degrade gradually because lost probes can simply cease contributing; a monolithic GHZ state can lose its entire collective advantage after one erasure.

Heralded generation changes what is known, not what it costs. A failed link attempt may be excluded from the estimator only if its elapsed time, source uses, memory aging, and any consumed probes remain in the resource ledger.

For quadratures with vacuum covariance I/2I/2, independent pure-loss channels transform a covariance matrix as

Vout=LVinL+12(I−L2),\boldsymbol V_{\rm out} = \boldsymbol L \boldsymbol V_{\rm in} \boldsymbol L + \frac12 \left( I-\boldsymbol L^2 \right),

where

L=diag⁡(η1,…,ηM)\boldsymbol L = \operatorname{diag} \left( \sqrt{\eta_1},\ldots,\sqrt{\eta_M} \right)

for one quadrature per node. Loss injects independent vacuum noise and also distorts the target supermode when the ηm\eta_m differ. The optimum splitter and electronic weights in a lossy network need not equal their lossless values. At fixed nonzero loss, ideal Heisenberg scaling generally crosses over to a weaker asymptotic law even when a finite-size advantage remains.

Let AmA_m be the random time at which node mm obtains its required link. The network state becomes usable only when all required resources are available, so its age distribution depends on a maximum or a scheduling policy, not only on the mean single-link latency. Early memories wait while slow links retry. If coherence decays as e−t/T2,me^{-t/T_{2,m}}, then the final contrast depends on the joint waiting-time distribution:

E[Cnet]∼C0E ⁣[∏me−Amwait/T2,m].\mathbb E[C_{\rm net}] \sim C_0 \mathbb E\!\left[ \prod_m e^{-A_m^{\rm wait}/T_{2,m}} \right].

Cutoffs can improve fidelity by discarding old states but reduce delivery rate. The optimum policy depends on the sensing objective and field correlation time; it is not determined by entanglement fidelity alone.

Distributed nodes must interrogate the same intended spacetime mode. In the frequency domain, one useful linear response is

q(ω)=∑m=1MwmκmHm(ω)e−iωτms(xm,ω),q(\omega) = \sum_{m=1}^{M} w_m\kappa_m H_m(\omega) e^{-i\omega\tau_m} s(\mathbf x_m,\omega),

where Hm(ω)H_m(\omega) is the node transfer function and τm\tau_m is its timing offset. A timing error rotates the weight by e−iωδτme^{-i\omega\delta\tau_m} and can mix a nominally rejected field mode into the target. Synchronization must be specified relative to the signal bandwidth, not only as a timestamp resolution.

Phase sensing also needs a frame in which local analysis angles are defined. Unknown local-oscillator phases can be exactly degenerate with the physical phases:

θmobs=θmsig−ϕmref.\theta_m^{\rm obs} = \theta_m^{\rm sig} - \phi_m^{\rm ref}.

A common laser, stabilized fibre link, two-way transfer protocol, calibrated comb, pilot tone, or reference pulse may supply the frame. Its noise and power are resources. Entanglement does not create a shared phase convention by itself.

Let AA denote an accepted network trial. The Fisher information in the full record decomposes as

Fqtrial=Fqflag+pAFq∣A+(1−pA)Fq∣Aˉ,F_q^{\rm trial} = F_q^{\rm flag} + p_A F_{q\mid A} + (1-p_A)F_{q\mid \bar A},

where

Fqflag=(∂qpA)2pA(1−pA).F_q^{\rm flag} = \frac{(\partial_qp_A)^2}{p_A(1-p_A)}.

When acceptance is independent of qq and rejected trials contain no useful information,

Fqtrial=pAFq∣A.F_q^{\rm trial} = p_AF_{q\mid A}.

The end-to-end information rate is

Iq:=FqtrialTc,\mathcal I_q := \frac{F_q^{\rm trial}}{T_c},

with cycle time TcT_c including state generation, herald communication, memory loading, synchronization, interrogation, readout, and reset. A distributed quantum advantage in averaging time requires

Grate:=IqentIqsep>1G_{\rm rate} := \frac{\mathcal I_q^{\rm ent}} {\mathcal I_q^{\rm sep}} > 1

under the same resource boundary. Conditional sensitivity can improve while information rate worsens if successful multipartite states are rare or slow.

The ledger should distinguish at least

Nsource⟶Ndistributed⟶Nencoding⟶Ndetected,N_{\rm source} \longrightarrow N_{\rm distributed} \longrightarrow N_{\rm encoding} \longrightarrow N_{\rm detected},

and record how many source and link attempts were required to produce each accepted sensing record.

Consider M=4M=4 equal-weight nodes and N=400N=400 ideal qubit probes per accepted trial. For one repetition, the three bounds are

protocol classVar⁡(q^)Δqproduct probes1/4000.050node-separable, locally entangled4/40020.0050inter-node GHZ1/40020.0025\begin{array}{c|c|c} \text{protocol class} & \operatorname{Var}(\widehat q) & \Delta q \\ \hline \text{product probes} & 1/400 & 0.050 \\ \text{node-separable, locally entangled} & 4/400^2 & 0.0050 \\ \text{inter-node GHZ} & 1/400^2 & 0.0025 \end{array}

Now suppose the inter-node state is usable on only 12%12\% of attempts, has C=0.80C=0.80, and takes twice the product-probe cycle time. Its information rate, in units of the product cycle time T0T_0, is

Iqent=0.12(0.80)2(400)22T0=6144T0.\mathcal I_q^{\rm ent} = \frac{ 0.12(0.80)^2(400)^2 }{2T_0} = \frac{6144}{T_0}.

The ideal product network has

Iqprod=400T0,\mathcal I_q^{\rm prod} = \frac{400}{T_0},

so the entangled protocol still has a factor 15.3615.36 information-rate gain over that baseline. But the ideal node-separable network has

Iqnode-sep=4002/4T0=40000T0.\mathcal I_q^{\rm node\text{-}sep} = \frac{400^2/4}{T_0} = \frac{40000}{T_0}.

The same experiment would therefore beat independent particles while failing to beat an ideal protocol with local entanglement at every node. Both statements can be true. A published claim must name which comparator is technologically and scientifically relevant.

The global fringe also repeats after

Δqwrap=2π400≃1.57×10−2rad.\Delta q_{\rm wrap} = \frac{2\pi}{400} \simeq 1.57\times10^{-2} \mathrm{rad}.

A broader prior needs another sensing tier; the local variance alone does not resolve the branch.

Two remote clocks can estimate a frequency difference while rejecting a shared interrogation oscillator. If the local phases after Ramsey time TT are

θm=(ωm−ωL)T,\theta_m = (\omega_m-\omega_L)T,

then

θ1−θ2=(ω1−ω2)T\theta_1-\theta_2 = (\omega_1-\omega_2)T

is independent of the common oscillator frequency ωL\omega_L in the ideal synchronous model. Correlation spectroscopy can exploit this cancellation without inter-node entanglement. A remote Bell state can further improve the quantum statistical term of the differential parity readout.

The claim boundary matters. Remote entanglement may improve a frequency-ratio measurement without improving either clock’s systematic shifts, uptime, time scale, or absolute realization of frequency. Optical Clocks owns those complete instrument and comparison budgets. Atomic Clocks for Quantum Estimation owns the information-rate and oscillator-tracking layer for a clock cycle.

An array can choose weights orthogonal to low-order nuisance profiles. For nodes at positions xmx_m, the constraints

∑mwm=0,∑mwmxm=0\sum_mw_m = 0, \qquad \sum_mw_mx_m = 0

reject a uniform offset and linear gradient, leaving sensitivity to curvature or another higher spatial moment. Entangled multilevel sensors can encode the desired signed weights into one protected coherence. This is useful when the nuisance amplitudes are large but their spatial forms are accurately known.

The same logic applies to coherent-field searches, magnetic arrays, inertial gradiometers, and spectroscopy networks. It does not guarantee an application advantage: the signal must remain coherent across the baseline and interrogation window, while sensor positions, coupling tensors, and timing must be known well enough that nuisance leakage stays below the claimed gain.

Continuous-variable optical networks can distribute one squeezed supermode to electro-optic, optomechanical, or interferometric transducers. Local homodyne currents are combined with weights matched to an average, edge difference, or beamforming mode. The architecture can be deterministic and high bandwidth, but its performance depends on transmission, phase-locked local oscillators, transducer gain, electronic covariance, and photons at the sample.

Discrete-variable photonic protocols can instead send path- or polarization-entangled photons through separated phase elements and recover a global phase from coincidence or parity statistics. Detection efficiency is decisive. A sub-shot-noise result conditioned on detecting every photon may disappear when launched photons and failed trials are included.

Some global states store the sensed phase only in joint correlations. A single-node reduced state may then reveal no information about qq, while authorized parties can reconstruct it from combined outcomes. This can support privacy against specified subsets of nodes.

Privacy is not automatic secrecy. A complete protocol must state which nodes, source, measurement station, and classical channels are trusted; what side information an adversary receives; and whether malicious devices can alter the encoding. Metrological privacy, cryptographic security, and device-independent certification are different claims.

Experiments have established several distinct milestones. Numerical gains below use each study’s stated resource convention and therefore should not be ranked as if they were one common benchmark.

ResultWhat was demonstratedBoundary and limitation
Guo et al. (2020)One squeezed optical mode was distributed into a four-node continuous-variable network to estimate the average of four phases deterministically. In one reported operating point, sensitivity was 0.099±0.0030.099\pm0.003 for the entangled network and 0.118±0.0020.118\pm0.002 for an optimized separable benchmark inferred from matched single-node measurements, with about 2.52.5 photons per sample and overall efficiency near 73.5%73.5\%.Laboratory optical phases and a local small-phase working regime; not a deployed field sensor or full phase map.
Xia et al. (2020)A configurable three-node RF-photonic network aligned multipartite quadrature correlations with average-amplitude and phase-difference tasks, reporting estimation variance 3.2±0.1 dB3.2\pm0.1\ \mathrm{dB} below its SQL.Laboratory electro-optic transduction; the demonstrated benchmark was a coherent classical separable network, not every possible locally squeezed network.
Liu et al. (2021)Mode- and particle-entangled photons estimated individual phases and an average phase, with reported error reductions up to 1.4 dB1.4\ \mathrm{dB} and 2.7 dB2.7\ \mathrm{dB} below shot noise.A proof-of-principle few-photon experiment; resource accounting is detection-based and should not be read as an unconditional launched-photon advantage.
Zhao et al. (2021)A discrete-variable field test reported an unconditional, no-postselection violation of the shot-noise limit by up to 0.916 dB0.916\ \mathrm{dB} across 240 m240\ \mathrm m; the apparatus also tested random phases with up to 10 km10\ \mathrm{km} of fibre.A two-node photonic phase task, not a general-purpose metropolitan sensor network. Loss and total efficiency remain central to scaling.
Nichol et al. (2022)A photonic link entangled two 88Sr+^{88}\mathrm{Sr}^{+} optical-clock ions separated by about 2 m2\ \mathrm m. The remote Bell protocol reduced frequency-comparison uncertainty by nearly 2\sqrt2 relative to independent single-ion measurements and by a factor near 22 relative to conventional correlation spectroscopy in the laser-dephasing regime.Proof of principle with two ions; absolute precision was below mature optical-clock comparisons, and generation time belongs in the rate comparison.
Malia et al. (2022)A shared quantum nondemolition measurement produced mode-entangled spin-squeezed atomic states in as many as four spatial modes. The article reported up to 4.5 dB4.5\ \mathrm{dB} better precision than a network without nonlocal entanglement and 11.6 dB11.6\ \mathrm{dB} relative to a stated projection-noise limit.A 2023 non-peer-reviewed critique disputes whether the plotted noise, response slope, and comparator establish those precision claims. The Nature article remains the version of record; the benchmark should be treated as disputed, not as settled network gain.
Bate et al. (2025)Three multilevel trapped-ion sensors encoded a quadratic spatial field while rejecting stronger constant and linear noise profiles. The reported entangled protocol had a factor 2.6(1)2.6(1) lower experimental RMSE than the separable protocol, quoted using the paper’s convention as a 4.1(2) dB4.1(2)\ \mathrm{dB} improvement, and outperformed the authors’ ideal bound for the comparable sensor-separable strategy.A controlled three-ion experiment over micrometre distances. The result validates structured-noise sensing, not long-baseline distribution or field readiness.

The record supports a measured conclusion: inter-node correlations can improve carefully chosen global estimators, and unconditional gains have been shown in small optical and atomic networks. It does not yet support a blanket claim that entanglement improves arbitrary field mapping or that a useful quantum sensor network can be inferred from link distance alone.

ClaimMinimum evidenceDoes not by itself establish
shared nonclassical stateentanglement, squeezing, or another nonclassicality witness across the declared node cutsensing gain
target-mode noise reductioncovariance or parity noise below a declared reference in the correct weighted moderetained signal response
sub-SQL estimatorcalibrated likelihood or response slope and lower error than a matched product-probe SQLinter-node advantage
inter-node advantagelower risk than the best allowed node-separable protocol with equal local resourcesinformation-rate gain
unconditional advantagefailures, loss, and rejected outcomes included at a declared source boundarywall-time advantage
field-task advantageend-to-end loss, bandwidth, timing, calibration, systematics, and comparator tested in the intended environmentuniversal superiority

Each rung requires new evidence. State tomography cannot replace a calibrated response curve. A sub-SQL conditional variance cannot replace failure accounting. A long entanglement link cannot replace an end-to-end sensing estimate.

Calling every sensor array quantum enhanced

Section titled “Calling every sensor array quantum enhanced”

Quantum mechanics is essential to each local device, but an array of independent atomic clocks or magnetometers is not thereby enhanced by inter-node quantum resources.

If local squeezing or local many-particle entanglement is allowed, the proper node-separable benchmark includes it. Beating coherent shot noise establishes a weaker claim.

Estimating one average and claiming a field map

Section titled “Estimating one average and claiming a field map”

A globally entangled state may concentrate information into one weighted functional while suppressing information about orthogonal modes. Report the actual estimand.

Treating covariance as an entanglement witness

Section titled “Treating covariance as an entanglement witness”

Common oscillators, environmental fields, electronics, and classical post-processing also create cross-covariances. Use a valid separability bound or an independently justified state certificate.

Discarded source attempts and lost probes can turn an apparent Heisenberg gain into a rate loss. State whether resources are counted at the source, sample, or detector.

An unknown local-oscillator phase is often indistinguishable from the signal. Reference distribution, pilot tones, phase locks, and synchronization belong in the model.

Varying node number while adding resources silently

Section titled “Varying node number while adding resources silently”

A 1/M1/M uncertainty law is not a quantum node-scaling advantage if the total number of photons, atoms, sources, or passes also grows with MM without being held fixed.

Section titled “Equating link distance with sensing performance”

Distributing entanglement over a long fibre is network-infrastructure evidence. A sensing claim additionally needs local encoding, calibrated readout, an estimator, and a matched error metric.

Assuming entanglement fixes systematic bias

Section titled “Assuming entanglement fixes systematic bias”

Entanglement can reshape statistical noise and reject modeled nuisance modes. It does not calibrate node positions, coupling tensors, clock shifts, wavefronts, or environmental corrections.

For a weighted functional

q=wTθ,q = \mathbf w^{\mathsf T}\boldsymbol\theta,

the ideal product-probe bound under optimized allocation is

Var⁡(q^)prod≥∥w∥12νN.\operatorname{Var}(\widehat q)_{\rm prod} \geq \frac{\|\mathbf w\|_1^2}{\nu N}.

Allowing ideal local entanglement but no inter-node entanglement gives

Var⁡(q^)node-sep≥(∑m∣wm∣2/3)3νN2.\operatorname{Var}(\widehat q)_{\rm node\text{-}sep} \geq \frac{ \left(\sum_m|w_m|^{2/3}\right)^3 }{\nu N^2}.

An ideal signed global GHZ protocol can attain

Var⁡(q^)global≥∥w∥12νN2\operatorname{Var}(\widehat q)_{\rm global} \geq \frac{\|\mathbf w\|_1^2}{\nu N^2}

for the declared global functional and local phase model. In realistic networks, contrast, success probability, and cycle time convert conditional Fisher information into

Iq=FqtrialTc.\mathcal I_q = \frac{F_q^{\rm trial}}{T_c}.

Entanglement is most compelling when it aligns a low-noise collective mode with the desired signal while rejecting identifiable nuisance modes. It is not generically optimal for learning every local parameter.

  1. T. J. Proctor, P. A. Knott, and J. A. Dunningham, “Multiparameter estimation in networked quantum sensors,” Physical Review Letters 120, 080501 (2018).
  2. Z. Eldredge, M. Foss-Feig, J. A. Gross, S. L. Rolston, and A. V. Gorshkov, “Optimal and secure measurement protocols for quantum sensor networks,” Physical Review A 97, 042337 (2018).
  3. W. Ge, K. Jacobs, Z. Eldredge, A. V. Gorshkov, and M. Foss-Feig, “Distributed quantum metrology with linear networks and separable inputs,” Physical Review Letters 121, 043604 (2018).
  4. Q. Zhuang, Z. Zhang, and J. H. Shapiro, “Distributed quantum sensing using continuous-variable multipartite entanglement,” Physical Review A 97, 032329 (2018).
  5. Z. Zhang and Q. Zhuang, “Distributed quantum sensing,” Quantum Science and Technology 6, 043001 (2021).
  6. X. Guo et al., “Distributed quantum sensing in a continuous-variable entangled network,” Nature Physics 16, 281–284 (2020).
  7. Y. Xia, W. Li, W. Clark, D. Hart, Q. Zhuang, and Z. Zhang, “Demonstration of a reconfigurable entangled radio-frequency photonic sensor network,” Physical Review Letters 124, 150502 (2020).
  8. S.-R. Zhao et al., “Field demonstration of distributed quantum sensing without post-selection,” Physical Review X 11, 031009 (2021).
  9. L.-Z. Liu et al., “Distributed quantum phase estimation with entangled photons,” Nature Photonics 15, 137–142 (2021).
  10. P. Kómár et al., “A quantum network of clocks,” Nature Physics 10, 582–587 (2014).
  11. E. S. Polzik and J. Ye, “Entanglement and spin squeezing in a network of distant optical lattice clocks,” Physical Review A 93, 021404(R) (2016).
  12. B. C. Nichol et al., “An elementary quantum network of entangled optical atomic clocks,” Nature 609, 689–694 (2022).
  13. B. K. Malia, Y. Wu, J. Martínez-Rincón, and M. A. Kasevich, “Distributed quantum sensing with mode-entangled spin-squeezed atomic states,” Nature 612, 661–665 (2022).
  14. L. P. McGuinness, “Matters Arising: Distributed quantum sensing with mode-entangled spin-squeezed atomic states,” arXiv:2302.00733 (2023), non-peer-reviewed critique.
  15. T. Qian, J. Bringewatt, I. Boettcher, P. Bienias, and A. V. Gorshkov, “Optimal measurement of field properties with quantum sensor networks,” Physical Review A 103, L030601 (2021).
  16. J. Bringewatt, A. Ehrenberg, T. Goel, and A. V. Gorshkov, “Optimal function estimation with photonic quantum sensor networks,” Physical Review Research 6, 013246 (2024).
  17. Q. Zhuang, J. Preskill, and L. Jiang, “Distributed quantum sensing enhanced by continuous-variable error correction,” New Journal of Physics 22, 022001 (2020).
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For product probes, minimize

V=∑mwm2nmV = \sum_m\frac{w_m^2}{n_m}

subject to nm>0n_m>0 and ∑mnm=N\sum_mn_m=N. Derive the optimum allocation and the minimum variance.

Solution

Introduce a multiplier λ\lambda:

L=∑mwm2nm+λ(∑mnm−N).\mathcal L = \sum_m\frac{w_m^2}{n_m} + \lambda \left(\sum_mn_m-N\right).

Stationarity gives

−wm2nm2+λ=0,-\frac{w_m^2}{n_m^2} + \lambda = 0,

so nm=∣wm∣/λn_m=|w_m|/\sqrt\lambda. Normalization yields

nm=N∣wm∣∑j∣wj∣.n_m = N\frac{|w_m|}{\sum_j|w_j|}.

Substitution gives

Vmin⁡=(∑m∣wm∣)2N=∥w∥12N.V_{\min} = \frac{(\sum_m|w_m|)^2}{N} = \frac{\|\mathbf w\|_1^2}{N}.

For ν\nu repetitions, divide this variance by ν\nu.

2. Optimize node-local Heisenberg resources

Section titled “2. Optimize node-local Heisenberg resources”

Allow ideal entanglement within each node, so the variance is

V=∑mwm2nm2.V = \sum_m\frac{w_m^2}{n_m^2}.

Find the optimal nmn_m at fixed ∑mnm=N\sum_mn_m=N.

Solution

Stationarity of

L=∑mwm2nm2+λ(∑mnm−N)\mathcal L = \sum_m\frac{w_m^2}{n_m^2} + \lambda \left(\sum_mn_m-N\right)

requires

−2wm2nm3+λ=0.-\frac{2w_m^2}{n_m^3} + \lambda = 0.

Hence nm∝∣wm∣2/3n_m\propto|w_m|^{2/3} and

nm=N∣wm∣2/3∑j∣wj∣2/3.n_m = N \frac{|w_m|^{2/3}}{\sum_j|w_j|^{2/3}}.

The minimum is

Vmin⁡=(∑m∣wm∣2/3)3N2.V_{\min} = \frac{(\sum_m|w_m|^{2/3})^3}{N^2}.

This comparator is stronger than the product-probe SQL whenever local many-particle entanglement is an allowed resource.

A network has M=3M=3 nodes and N=120N=120 total probes. Compute the ideal single-trial standard deviations for product probes, locally entangled but node-separable probes, and one inter-node GHZ protocol when estimating the equal average.

Solution

For wm=1/3w_m=1/3, the variances are

Vprod=1120,Vnode-sep=31202,Vglobal=11202.V_{\rm prod} = \frac{1}{120}, \qquad V_{\rm node\text{-}sep} = \frac{3}{120^2}, \qquad V_{\rm global} = \frac{1}{120^2}.

Therefore

Δqprod≃9.13×10−2,\Delta q_{\rm prod} \simeq 9.13\times10^{-2}, Δqnode-sep≃1.44×10−2,Δqglobal≃8.33×10−3.\Delta q_{\rm node\text{-}sep} \simeq 1.44\times10^{-2}, \qquad \Delta q_{\rm global} \simeq 8.33\times10^{-3}.

The global protocol improves variance by a factor 33 over the ideal node-separable protocol, but by a factor 120120 over independent particles.

4. Average and difference covariance modes

Section titled “4. Average and difference covariance modes”

Two calibrated readouts have covariance

Σ=σ2(1ρρ1).\boldsymbol\Sigma = \sigma^2 \begin{pmatrix} 1 & \rho\\ \rho & 1 \end{pmatrix}.

Find the variances of q+=(θ1+θ2)/2q_+=(\theta_1+\theta_2)/2 and q−=(θ1−θ2)/2q_-=(\theta_1-\theta_2)/2. Which sign of correlation helps each task?

Solution

Using V=wTΣwV=\mathbf w^{\mathsf T}\boldsymbol\Sigma\mathbf w gives

Var⁡(q^+)=σ22(1+ρ),\operatorname{Var}(\widehat q_+) = \frac{\sigma^2}{2}(1+\rho),

and

Var⁡(q^−)=σ22(1−ρ).\operatorname{Var}(\widehat q_-) = \frac{\sigma^2}{2}(1-\rho).

Negative covariance helps the average, whereas positive covariance helps the difference. “More correlation” is not a task-independent resource; its sign and orientation matter.

Three nodes lie at x=−1,0,1x=-1,0,1. Their phases follow

θ(x)=a+bx+cx2.\theta(x) = a+bx+cx^2.

Find weights w\mathbf w such that c^=∑mwmθ(xm)\widehat c=\sum_mw_m\theta(x_m) rejects aa and bb and has unit response to cc. If independent readout noise at each node has variance σ2\sigma^2, what is Var⁡(c^)\operatorname{Var}(\widehat c)?

Solution

The constraints are

w1+w2+w3=0,w_1+w_2+w_3 = 0, −w1+w3=0,w1+w3=1.-w_1+w_3 = 0, \qquad w_1+w_3 = 1.

Thus

w=(12,−1,12).\mathbf w = \left( \frac12,-1,\frac12 \right).

For independent equal noise,

Var⁡(c^)=σ2(14+1+14)=32σ2.\operatorname{Var}(\widehat c) = \sigma^2 \left( \frac14+1+\frac14 \right) = \frac32\sigma^2.

Quantum covariance engineering can reduce this target-mode variance, but the unbiasedness constraints still come from geometry and calibration.

6. Loss threshold for an all-or-nothing GHZ trial

Section titled “6. Loss threshold for an all-or-nothing GHZ trial”

An NN-probe GHZ state has ideal conditional Fisher information N2N^2. Every probe survives independently with probability η\eta, and a trial is rejected if any probe is lost. Compare its unconditional Fisher information with the NN of an ideal product trial. Derive the minimum η\eta for a gain and evaluate it for N=20N=20.

Solution

The GHZ survival probability is ηN\eta^N, so

FGHZtrial=ηNN2.F_{\rm GHZ}^{\rm trial} = \eta^NN^2.

It exceeds Fprod=NF_{\rm prod}=N only if

ηN>1N,\eta^N > \frac1N,

or

η>N−1/N.\eta > N^{-1/N}.

For N=20N=20,

η>20−1/20≃0.861.\eta > 20^{-1/20} \simeq 0.861.

This simplified threshold ignores contrast and cycle-time penalties, which would raise the required efficiency.

An entangled protocol succeeds with probability pA=0.10p_A=0.10, has conditional Fisher information Fq∣A=1000F_{q\mid A}=1000, and takes cycle time 5T05T_0. Rejected trials carry no information. A separable protocol has Fq=40F_q=40 every cycle and cycle time T0T_0. Which protocol has the larger information rate?

Solution

The entangled information per attempted trial is

Fqtrial=pAFq∣A=100.F_q^{\rm trial} = p_AF_{q\mid A} = 100.

Its information rate is

Iqent=1005T0=20T0.\mathcal I_q^{\rm ent} = \frac{100}{5T_0} = \frac{20}{T_0}.

The separable rate is

Iqsep=40T0.\mathcal I_q^{\rm sep} = \frac{40}{T_0}.

The entangled protocol has much larger information in a successful record but only half the wall-time information rate.

8. Timing leakage into a differential channel

Section titled “8. Timing leakage into a differential channel”

Two nodes estimate a difference with weights (1/2,−1/2)(1/2,-1/2). A common nuisance is s(t)=Acos⁡(ωt)s(t)=A\cos(\omega t), but the interrogation centers differ by δτ=τ1−τ2\delta\tau=\tau_1-\tau_2. Show that the residual differential signal is at most approximately Aω∣δτ∣/2A\omega|\delta\tau|/2 for small timing mismatch.

Solution

The nuisance contribution is

qleak=A2[cos⁡(ωτ1)−cos⁡(ωτ2)].q_{\rm leak} = \frac A2 \left[ \cos(\omega\tau_1) - \cos(\omega\tau_2) \right].

Writing τˉ=(τ1+τ2)/2\bar\tau=(\tau_1+\tau_2)/2 and using the cosine-difference identity gives

qleak=−Asin⁡(ωτˉ)sin⁡ ⁣(ωδτ2).q_{\rm leak} = -A \sin(\omega\bar\tau) \sin\!\left( \frac{\omega\delta\tau}{2} \right).

For ∣ωδτ∣≪1|\omega\delta\tau|\ll1,

∣qleak∣≲Aω∣δτ∣2.|q_{\rm leak}| \lesssim \frac{A\omega|\delta\tau|}{2}.

The required synchronization accuracy therefore depends on nuisance amplitude and frequency as well as on the target uncertainty.