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Weak Measurements

A weak measurement is a measurement that extracts only a small amount of information in a single trial and produces correspondingly small conditional backaction in that trial. Repeating the measurement many times, or taking a continuous-time limit, can still produce strong information and substantial cumulative disturbance.

The safe definition is operational:

weakmeans low signal-to-noise per shot,not disturbance-free.\text{weak} \quad \text{means low signal-to-noise per shot,} \quad \text{not disturbance-free.}

Weak measurements are best specified by an instrument or by an explicit system-pointer model. A POVM may be unsharp while the underlying instrument is still highly disturbing, so the phrase “weak” should not be inferred from effects alone.

An unsharp measurement has nonprojective effects. A weak measurement is a regime of small information gain and small state change per measurement step.

For the qubit unsharp σz\sigma_z effects

E±=12(I±ϵσz),0≤ϵ≪1,E_\pm = \frac{1}{2} \left( I\pm\epsilon\sigma_z \right), \qquad 0\le\epsilon\ll1,

a gentle square-root instrument has measurement operators

M±=12(1±ϵ P++1∓ϵ P−),M_\pm = \sqrt{\frac{1}{2}} \left( \sqrt{1\pm\epsilon}\,P_+ + \sqrt{1\mp\epsilon}\,P_- \right),

where P±=(I±σz)/2P_\pm=(I\pm\sigma_z)/2. Each result only slightly biases the state toward one σz\sigma_z eigenspace.

The associated nonselective channel multiplies the off-diagonal element in the σz\sigma_z basis by

1−ϵ2≈1−ϵ22.\sqrt{1-\epsilon^2} \approx 1-\frac{\epsilon^2}{2}.

Thus the unread disturbance is second order in the small measurement strength for this instrument. That gentle scaling is an instrument property, not a consequence of the POVM alone. See Unsharp Measurements.

The standard von Neumann pointer model makes the weak regime geometric. Let the measured observable be

A=∑aaPa,A=\sum_a aP_a,

and let a pointer have coordinate QQ and conjugate momentum PQP_Q. During the measurement interaction,

Hint(t)=g(t)A⊗PQ.H_{\mathrm{int}}(t) = g(t)A\otimes P_Q.

Define the integrated coupling

κ=∫dt g(t).\kappa=\int dt\,g(t).

The corresponding unitary is

U=exp⁡ ⁣(−iℏκA⊗PQ).U = \exp \!\left( -\frac{i}{\hbar}\kappa A\otimes P_Q \right).

If the system is in an eigenstate ∣a⟩\lvert a\rangle and the initial pointer wavefunction is ϕ(q)\phi(q), the interaction shifts the pointer:

∣a⟩ϕ(q)⟼∣a⟩ϕ(q−κa).\lvert a\rangle\phi(q) \longmapsto \lvert a\rangle\phi(q-\kappa a).

The measurement is weak when the shifts between relevant eigenvalues are small compared with the pointer width:

∣κ(a−b)∣≪ΔQ.|\kappa(a-b)| \ll \Delta Q.

Then the pointer distributions overlap strongly. A single readout gives little information about aa, and the conditional state changes only slightly.

If the pointer coordinate is read and the outcome is qq, the induced system measurement operator is formally

M(q)=⟨q∣U∣ϕ⟩=ϕ(q−κA),M(q) = \langle q|U|\phi\rangle = \phi(q-\kappa A),

where the last expression is functional calculus for the observable AA. The probability density is

p(q)=Tr⁡ ⁣[M(q)†M(q)ρ].p(q) = \operatorname{Tr} \!\left[ M(q)^\dagger M(q)\rho \right].

The conditional state after observing qq is

ρq=M(q)ρM(q)†p(q).\rho_q = \frac{M(q)\rho M(q)^\dagger} {p(q)}.

When κ\kappa is small relative to the pointer width, nearby eigenvalues of AA produce heavily overlapping likelihoods. The measurement is informative only statistically over many repetitions or after combining it with other conditioning.

Weak measurements are weak per step, not weak in total. If the same weak unread square-root qubit measurement is repeated NN times and the outcomes are ignored, the coherence factor is

(1−ϵ2)N≈exp⁡ ⁣(−Nϵ22)\left(\sqrt{1-\epsilon^2}\right)^N \approx \exp\!\left(-\frac{N\epsilon^2}{2}\right)

for small ϵ\epsilon. A large number of weak steps can therefore produce strong dephasing.

The record also accumulates information. For a small bias ϵ\epsilon, the signal-to-noise ratio between the two σz\sigma_z eigenstates grows like

ϵN.\epsilon\sqrt{N}.

Thus NN of order 1/ϵ21/\epsilon^2 weak trials can reveal order-one information. The cumulative backaction appears on the same scale.

Continuous measurement is the limit of many weak instruments applied over short time steps. A common scaling is

ϵ2∼Γm dt,\epsilon^2 \sim \Gamma_m\,dt,

where Γm\Gamma_m is a measurement rate. Individual steps become infinitesimal, but the accumulated record over finite time carries information.

For a Hermitian monitored observable AA, one common diffusive-record convention has a record increment

drt=2Γm ⟨A⟩c dt+dWt,dr_t = 2\sqrt{\Gamma_m}\, \langle A\rangle_c\,dt + dW_t,

where dWtdW_t is a Wiener increment and ⟨A⟩c=Tr⁡(Aρc)\langle A\rangle_c=\operatorname{Tr}(A\rho_c). The conditioned state obeys a stochastic master equation whose measurement part has the schematic form

dρc=ΓmD[A]ρc dt+Γm H[A]ρc dWt,d\rho_c = \Gamma_m\mathcal D[A]\rho_c\,dt + \sqrt{\Gamma_m}\, \mathcal H[A]\rho_c\,dW_t,

with

D[A]ρ=AρA−12{A2,ρ},\mathcal D[A]\rho = A\rho A - \frac{1}{2} \{A^2,\rho\},

and, for Hermitian AA,

H[A]ρ=Aρ+ρA−2Tr⁡(Aρ)ρ.\mathcal H[A]\rho = A\rho+\rho A - 2\operatorname{Tr}(A\rho)\rho.

Different communities use different factors of 22 in Γm\Gamma_m and in the record. The invariant point is the scaling: weak information per short interval plus stochastic conditioning yields continuous monitoring. See Stochastic Master Equations and Diffusive Trajectories.

Weak values arise when a weak measurement is combined with preselection and postselection. Prepare an initial state ∣ψi⟩\lvert\psi_i\rangle, weakly couple a pointer to observable AA, and later keep only runs in which a final measurement finds ∣ψf⟩\lvert\psi_f\rangle.

The weak value is

Aw=⟨ψf∣A∣ψi⟩⟨ψf∣ψi⟩,A_w = \frac{ \langle\psi_f|A|\psi_i\rangle }{ \langle\psi_f|\psi_i\rangle },

provided the denominator is nonzero.

In the weak-coupling limit, the mean pointer shift in the postselected ensemble is proportional to Re⁡Aw\operatorname{Re}A_w, while the conjugate pointer shift is related to Im⁡Aw\operatorname{Im}A_w in standard Gaussian-pointer conventions.

Weak values can be complex and can lie outside the spectrum of AA. That is not a single-shot detector reading and not direct evidence that the system possessed an anomalous pre-existing value. It is a conditional statistical quantity arising from weak coupling plus postselection. The canonical treatment of the weak-value quantity itself is Weak Values.

Postselection changes the ensemble. A weak measurement without postselection estimates ordinary expectation values. A weak measurement with postselection estimates a conditional response of the pointer in the retained subensemble.

If ⟨ψf∣ψi⟩\langle\psi_f|\psi_i\rangle is small, the weak value can become large. But the postselection probability is then small, so statistical uncertainty and experimental imperfections become crucial. Large weak values are not free amplification; they come with sampling costs and sensitivity to background errors.

This is the main caution:

weak-value formulasare statistical response formulas,not licenses to ignore measurement modeling.\text{weak-value formulas} \quad \text{are statistical response formulas,} \quad \text{not licenses to ignore measurement modeling.}

A weak measurement can be gentle in the measured trial, but it still correlates system and pointer. If the pointer is ignored, the system experiences a nonselective channel. If the pointer is read, the system is conditioned on a noisy outcome. If a postselection is then applied, the retained ensemble is biased by both the weak readout and the final selection.

Disturbance can be small enough to justify a perturbative expansion, but it is not absent. The validity of a weak-measurement calculation depends on:

  1. the coupling strength relative to pointer width;
  2. the number of repetitions or total monitoring time;
  3. whether the pointer record is retained or ignored;
  4. whether postselection is rare;
  5. whether higher-order backaction terms are negligible for the claimed result.

Weak per step does not mean disturbance-free. Backaction can accumulate over many repetitions or become important after postselection.

A weak measurement is not merely a sharp measurement with bad classical readout. It requires a weak system-pointer correlation or an instrument with small per-step state change.

Weak values can be outside the eigenvalue range and can be complex. They are conditional pointer-response quantities, not ordinary eigenvalues revealed in a single run.

Large weak values often occur when the postselected state is nearly orthogonal to the preselected state. The retained data set can then be rare and statistically fragile.

In continuous measurement, both the information gain and the noise scale with dtdt. Treating the record increment like an ordinary deterministic small number gives the wrong stochastic equation.

For

M±=12(1±ϵ P++1∓ϵ P−),M_\pm = \sqrt{\frac{1}{2}} \left( \sqrt{1\pm\epsilon}\,P_+ + \sqrt{1\mp\epsilon}\,P_- \right),

show that the effects are E±=(I±ϵσz)/2E_\pm=(I\pm\epsilon\sigma_z)/2.

Solution

Since P+P−=0P_+P_-=0 and P±2=P±P_\pm^2=P_\pm,

M+†M+=1+ϵ2P++1−ϵ2P−.M_+^\dagger M_+ = \frac{1+\epsilon}{2}P_+ + \frac{1-\epsilon}{2}P_-.

Using P±=(I±σz)/2P_\pm=(I\pm\sigma_z)/2, this becomes

M+†M+=12(I+ϵσz).M_+^\dagger M_+ = \frac{1}{2} \left( I+\epsilon\sigma_z \right).

Similarly,

M−†M−=12(I−ϵσz).M_-^\dagger M_- = \frac{1}{2} \left( I-\epsilon\sigma_z \right).

If each unread weak step multiplies ρ01\rho_{01} by 1−ϵ2\sqrt{1-\epsilon^2}, show that after NN identical steps the factor is approximately exp⁡(−Nϵ2/2)\exp(-N\epsilon^2/2) for small ϵ\epsilon.

Solution

After NN steps, the factor is

(1−ϵ2)N=exp⁡ ⁣[N2log⁡(1−ϵ2)].\left(\sqrt{1-\epsilon^2}\right)^N = \exp \!\left[ \frac{N}{2} \log(1-\epsilon^2) \right].

For small ϵ\epsilon,

log⁡(1−ϵ2)≈−ϵ2.\log(1-\epsilon^2)\approx-\epsilon^2.

Therefore

(1−ϵ2)N≈exp⁡ ⁣(−Nϵ22).\left(\sqrt{1-\epsilon^2}\right)^N \approx \exp\!\left(-\frac{N\epsilon^2}{2}\right).

In the pointer model, explain why ∣κ(a−b)∣≪ΔQ|\kappa(a-b)|\ll\Delta Q is the weak-measurement condition for eigenvalues aa and bb.

Solution

The coupling shifts the pointer wavepacket by κa\kappa a for eigenvalue aa and by κb\kappa b for eigenvalue bb. The separation between those pointer packets is ∣κ(a−b)∣|\kappa(a-b)|. If this separation is much smaller than the initial pointer width ΔQ\Delta Q, the distributions overlap strongly. A single pointer reading then gives little information about which eigenvalue was present, and the measurement is weak for that pair of alternatives.

Let A=σzA=\sigma_z, ∣ψi⟩=∣+x⟩=(∣0⟩+∣1⟩)/2\lvert\psi_i\rangle=\lvert+x\rangle=(\lvert0\rangle+\lvert1\rangle)/\sqrt2, and

∣ψf⟩=∣0⟩−α∣1⟩1+α2,0≤α<1.\lvert\psi_f\rangle = \frac{\lvert0\rangle-\alpha\lvert1\rangle} {\sqrt{1+\alpha^2}}, \qquad 0\le\alpha\lt1.

Compute AwA_w and explain why it can exceed 11.

Solution

The denominator is

⟨ψf∣ψi⟩=1−α2(1+α2).\langle\psi_f|\psi_i\rangle = \frac{1-\alpha} {\sqrt{2(1+\alpha^2)}}.

The numerator is

⟨ψf∣σz∣ψi⟩=1+α2(1+α2).\langle\psi_f|\sigma_z|\psi_i\rangle = \frac{1+\alpha} {\sqrt{2(1+\alpha^2)}}.

Therefore

Aw=1+α1−α.A_w = \frac{1+\alpha}{1-\alpha}.

As α\alpha approaches 11, the preselected and postselected states become nearly orthogonal, the denominator becomes small, and AwA_w can exceed the eigenvalue range [−1,1][-1,1]. This is a postselected weak-response quantity, not a single-shot eigenvalue.

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