Abstract
Measurements are crucial in quantum mechanics, for fundamental research as well as for applicative fields like quantum metrology, quantumenhanced measurements and other quantum technologies. In the recent years, weakinteractionbased protocols like Weak Measurements and Protective Measurements have been experimentally realized, showing peculiar features leading to surprising advantages in several different applications. In this work we analyze the validity range for such measurement protocols, that is, how the interaction strength affects the weak value extraction, by measuring different polarization weak values on heralded single photons. We show that, even in the weak interaction regime, the coupling intensity limits the range of weak values achievable, setting a threshold on the signal amplification effect exploited in many weak measurement based experiments.
Introduction
The fundamental role of measurement in quantum mechanics is undisputed^{1}, since it is the process in which some of the distinctive traits of the quantum world with respect to the classical one appear: e.g., the fact that quantum states collapse in a specific eigenstate of the observable (corresponding to the measured eigenvalue) when a strong measurement (described by a projection operator) is performed, causing the impossibility to measure noncommuting observables on the same particle.
However, in recent years a new paradigm of quantum measurement emerged, in which the coupling strength between the measured quantum state and the measurement system is weak enough to prevent the wave function collapse (at the cost of extracting only a small amount of information from a single measurement). It is the case of Weak Measurements (WMs), introduced in^{2,3} and firstly realized in^{4,5,6}, and Protective Measurements (PMs), originally proposed within the debate on the reality of the wave function^{7} and recently realized for the first time^{8}.
WMs can give rise to anomalous (imaginary and/or unbounded) values, whose real part is regarded as a conditional average of the observable in the zerodisturbance limit^{9}, while the imaginary one is related to the disturbance of the measuring pointer during the measurement^{10}. Beyond having inspired a significant analysis of the meaning of quantum measurement^{11,12,13,14,15,16,17,18}, they have been used both to address foundational problems^{19}, like macrorealism^{20,21,22} and contextuality^{23,24,25}, and as a novel, impressive tool for quantum metrology and related quantum technologies allowing highprecision measurements (at least in presence of specific noises^{26,27}), as the tiny spin Hall effect^{6} or small beam deflections^{28,29,30,31} and characterization of quantum states^{32,33}. Furthermore, the absence of wave function collapse in WMs allows performing sequential measurements of even noncommuting observables on the same particle^{34,35,36,37}, a task forbidden within the strong measurement framework in quantum mechanics.
On the other hand, PMs combine the weak interaction typical of WMs with some protection mechanism preserving the initial state from decoherence. Although a very controversial and debated topic from the foundational perspective^{38,39,40,41,42,43,44,45,46,47,48}, PMs have demonstrated unprecedented measurement capability, allowing to extract the quantum expectation value of an observable in a single measurement on a single (protected) particle^{8}, a task usually forbidden in quantum mechanics.
Both of these protocols require a von Neumann interaction with a very weak coupling between the observable to be measured and the pointer observable, rising the issue of when the regime of weak interaction approximation can be considered valid^{49,50}. For instance, this is of the utmost relevance specially when dealing with anomalous weak values, for which the weakness of the von Neumann interaction is crucial for the reliability of the measurement, giving rise to a signal amplification effect already demonstrated in several experiments^{6,26,27,28,29,30,31}.
Up to now, a generic theoretical discussion of this point has been carried out in^{51,52,53,54,55,56,57,58,59}, while a few papers^{60,61,62,63,64,65} have afforded an experimental investigation of this issue for specific physical systems. In this work we aim at investigating the specific case of polarization weak measurements, both for its widespread application^{66,67,68,69,70} and as an emblematic example of general considerations. For this purpose, we have realized a singlephotonbased experiment studying the response of the weak value measurement process in different conditions and observing, for a given interaction strength, the limits in which the expected weak value can be accurately extracted. Up to our knowledge, this is the first time for such an experiment to be run at the single particle level, the regime which WMs really belong to.
We show how the von Neumann coupling intensity intrinsically provides some boundaries on the range of weak values that one is able to determine without abandoning the weak interaction approximation, setting, as a consequence, a threshold on the signal amplification effect mentioned above.
Theoretical framework
The weak value of an observable \(\hat{A}\) is defined as \({\langle \hat{A}\rangle }_{w}=\frac{\langle {{\psi }}_{f}\hat{A}{{\psi }}_{i}\rangle }{\langle {{\psi }}_{f}{{\psi }}_{i}\rangle }\), where ψ_{ i }〉 and ψ_{ f }〉 are the pre and postselected quantum states, respectively^{2}. To extract the weak value, one usually implements a von Neumann indirect measurement coupling the observable of interest (OoI) \(\hat{A}\) to a pointer observable \(\hat{P}\) by means of the unitary operation \(\hat{U}={e}^{ig\hat{A}\otimes \hat{P}}\), being g the von Neumann coupling strength. After a postselection onto the state ψ_{ f }〉, realized by the projector \({\hat{{\rm{\Pi }}}}_{f}={{\psi }}_{f}\rangle \langle {{\psi }}_{f}\), the information on the OoI is obtained by measuring the meter observable \(\hat{Q}\), canonically conjugated with the pointer \(\hat{P}\).
Let us focus on the case of a single qubit, and take as OoI a projection operator of the form \(\hat{{A}}={{\rm{\psi }}}_{A}\rangle \langle {\psi }_{A}\). Considering the initial state \({{\rm{\psi }}}_{i}\rangle ={\psi }_{i}\rangle \otimes \varphi (q)\rangle \), after the von Neumann interaction and the subsequent postselection the final state is:
being \(z=\langle {{\psi }}_{f}{{\psi }}_{i}\rangle \) the internal product between the pre and postselected state.
Then, considering as initial condition \(\langle {\varphi }(q)\hat{Q}{\varphi }(q)\rangle =0\), the expectation value of the meter observable \(\hat{Q}\) onto the final state can be written as:
In the limit of weak interaction (g → 0), the first perturbative order of the right term in Eq. (2) is:
Hence, restricting ourselves to the case of real weak values, Eq. (2) gives:
showing how the (real) weak value of our OoI A can be obtained by a measurement of the meter Q, canonically conjugated with the pointer P. Going further in the series expansion, one finds that the contribution at the second order is null, so the next nontrivial contribution scales as g^{3}.
In our experiment we extract the weak value of the polarization of single photons, collimated in a Gaussian mode \({\varphi }(q)\rangle =\int dqf(q)q\rangle \), with \(f(q)={\mathrm{(2}\pi {\sigma }^{2})}^{\frac{1}{4}}\,\exp (\frac{{q}^{2}}{4{\sigma }^{2}})\). The \(Im[{\langle \hat{A}\rangle }_{w}]=0\) constraint is satisfied by restricting to pre and postselected states of the form \({{\psi }}_{j}\rangle =\,\cos \,{{\theta }}_{j}H\rangle +\,\sin \,{{\theta }}_{j}V\rangle \), where H (V) indicates the horizontal (vertical) polarization and j = i, f the pre and postselected state. As pointer observable we choose the transverse momentum \({\hat{P}}_{Q}\) in the direction Q (orthogonal to the photon propagation direction), \(\hat{Q}\) being our meter observable.
Experimental implementation
The single photons exploited in our experiment are produced by a heralded singlephoton source^{71,72} in which a 76 MHz Ti:Sapphire modelocked laser at 796 nm is frequency doubled via second harmonic generation and then injected into a 5 mm thick LiIO_{3} nonlinear crystal, generating photon pairs via typeI Parametric DownConversion (PDC), as reported in Fig. 1.
The idler photon (λ_{ i } = 920 nm) is filtered by an interference filter (IF), coupled to a single mode fiber (SMF) and detected by a silicon singlephoton avalanche diode (SiSPAD). A click from the SiSPAD heralds the presence of the signal photon (λ_{ s } = 702 nm) in the correlated branch. Such photon passes through an IF, then is SMF coupled and addressed, collimated in a Gaussian mode, to the open air path where the WMs take place. We have verified our single photon emission by measuring the antibunching parameter^{73} of our source, obtaining a value of 0.13(1) without any background/darkcount subtraction.
In such path, the heralded single photon is prepared in the linearlypolarized state \({{\psi }}_{i}\rangle =\frac{1}{\sqrt{2}}(H\rangle +V\rangle )\) by means of a polarizing beam splitter (PBS) followed by a half wave plate. After the state preparation, the photon encounters a pair of thin birefringent crystals, responsible for the weak interactions. The first birefringent crystal (BC_{ V }) presents an extraordinary (e) optical axis lying in the YZ plane, with an angle of π/4 with respect to the Z direction. The spatial walkoff induced on the photons by BC_{ V } slightly shifts the verticallypolarized ones, separating horizontal and verticalpolarization paths along the Y direction and causing the initial state ψ_{ i }〉 to be affected by a small amount of decoherence. This element realizes the first (weak) interaction \({\hat{U}}_{V}={e}^{i{a}_{y}{\hat{{\rm{\Pi }}}}_{V}\otimes {\hat{P}}_{y}}\), coupling the observable under test (i.e. the vertical polarization \({\hat{{\rm{\Pi }}}}_{V}=V\rangle \langle V)\) to the pointer observable, the transverse momentum along the Y direction \({\hat{P}}_{y}\).
Then, the photon goes through the second birefringent crystal (BC_{ H }), identical to the first one, but with the eaxis lying in the XZ plane. Here, the photons experiencing the spatial walkoff are the horizontallypolarized ones. They are shifted along the X direction and the initial polarization state undergoes the same decoherence induced by the passage in BC_{ V }. This way, the second (weak) interaction \({\hat{U}}_{H}={e}^{i{a}_{x}{\hat{{\rm{\Pi }}}}_{H}\otimes {\hat{P}}_{x}}\) occurs. This configuration allows measuring simultaneously the weak values of the two orthogonal polarizations \({\hat{{\rm{\Pi }}}}_{V}\) and \({\hat{{\rm{\Pi }}}}_{H}\), at the same time selfcompensating the unwanted temporal walkoff induced by the two interactions.
After the two birefringent crystals, the photon undergoes the postselection, that is, a projection onto the final state ψ_{ f }〉 realized by a half wave plate followed by a PBS.
The final photon detection is performed by a spatial resolving singlephoton detector prototype, i.e. a twodimensional array made of 32 × 32 “smart pixels” (each hosting a SPAD detector with dedicated frontend electronics for counting and timing single photons) operating in parallel with a global shutter readout^{74}. Each count by the SiSPAD on the heralding arm triggers a 6 ns detection window in each pixel of the SPAD array, in order to heavily decrease the dark count rate and improve the signaltonoise ratio.
We perform two different acquisitions, respectively with 1 mm and 2.5 mm thick birefringent crystals, in order to change the coupling strength of the weak interactions experienced by the single photons. In each acquisition, we variate the postselection state and measure different weak values, observing the behaviour of the meter variables with respect to the weak values theoretically predicted.
Results and Conclusions
For each pair of birefringent crystals, we perform an initial system calibration to determine the von Neumann coupling intensity g, obtaining for the 1mm long crystals a_{ x } = a_{ y } = 0.7 pixels (px), while a_{ x } = 1.9 px and a_{ y } = 1.7 px for the 2.5mm long ones (the small discrepancy between a_{ x } and a_{ y } is due to a slight mismatch in the birefringent crystals cut). Considering that our single photons are collimated in a Gaussian distribution whose width parameter is σ = 4.3 px, the two birefringent crystal pairs induce respectively an interaction strength of \({g}_{x}={g}_{y}={a}_{y}/\sigma \simeq 0.16\) and \({g}_{y}={a}_{y}/\sigma \simeq 0.40\) and \({g}_{x}={a}_{x}/\sigma \simeq 0.45\). These conditions should still lie within the weak interaction regime, since for all of them \({g}^{2}\ll 1\).
The results obtained with the 1mm and 2.5mm birefringent crystal pairs are reported in Figs 2 and 3, respectively. In each of these figures, plots (a) and (b) report the behavior of the meter observables \(\langle \hat{X}\rangle \) and \(\langle \hat{Y}\rangle \) with respect to the theoretical weak values associated to them (\({\langle {\hat{{\rm{\Pi }}}}_{H}\rangle }_{w}\) and \({\langle {\hat{{\rm{\Pi }}}}_{V}\rangle }_{w}\), respectively). The orange (purple) dots are the measured values of \(\langle \hat{X}\rangle \) (\(\langle \hat{Y}\rangle \)), the solid curve represents the exact solution of Eq. (2) while the dotted line and the dashed curve indicate respectively the first order approximation, corresponding to the weak value \({\langle {\hat{{\rm{\Pi }}}}_{H}\rangle }_{w}\) (\({\langle {\hat{{\rm{\Pi }}}}_{V}\rangle }_{w}\)), and the third order one in the \({g}^{2}\ll 1\) limit (we remind the reader that the second order approximation gives null contribution).
As visible in Fig. 2, obtained in the condition \(g\simeq 0.16\) with the 1 mm birefringent crystals, the weak value approximation is valid for a good range of anomalous values, that is, for \({\langle {\hat{{\rm{\Pi }}}}_{H}\rangle }_{w},{\langle {\hat{{\rm{\Pi }}}}_{V}\rangle }_{w}\in [\mathrm{1.5,}\,2.5]\) (region I). Outside this interval, the data start following the third order approximation and the exact solution, almost indistinguishable in the investigated range (region II). This means that, outside region I, a bias begins to affect our weak value estimation.
The situation becomes different when we switch to the 2.5mm long BC_{ H } and BC_{ V }, increasing the interaction strength almost to the border of the weak interaction regime. By looking at Fig. 3, we can identify three regions: region I, corresponding to \({\langle {\hat{{\rm{\Pi }}}}_{H}\rangle }_{w},{\langle {\hat{{\rm{\Pi }}}}_{V}\rangle }_{w}\in [\mathrm{0.7,}\,1.7]\), for which the meter observables still follow the weak value approximation; region II, for \({\langle {\hat{{\rm{\Pi }}}}_{H}\rangle }_{w},{\langle {\hat{{\rm{\Pi }}}}_{V}\rangle }_{w}\in [\mathrm{1.2,}0.7]\vee \mathrm{[1.7},\,\mathrm{2.2]}\), in which the third order approximation (dashed line) is still valid; region III (absent in Fig. 2), corresponding to \({\langle {\hat{{\rm{\Pi }}}}_{H}\rangle }_{w},{\langle {\hat{{\rm{\Pi }}}}_{V}\rangle }_{w} < 1.2\vee {\langle {\hat{{\rm{\Pi }}}}_{H}\rangle }_{w},{\langle {\hat{{\rm{\Pi }}}}_{V}\rangle }_{w} > \,2.2\), in which the exact solution assumes a quasiasymptotic form and both approximations fail. In this last region, our meter observables \(\langle \hat{X}\rangle \) and \(\langle \hat{Y}\rangle \) remain basically constant with respect to \({\langle {\hat{{\rm{\Pi }}}}_{H}\rangle }_{w}\) and \({\langle {\hat{{\rm{\Pi }}}}_{V}\rangle }_{w}\), hence it is not possible anymore to extract the weak value.
In summary, while in region I in principle one can safely estimate the weak value, in region II the bias due to the finite interaction intensity already affects such estimation, completely forbidding it in region III. This means that the signal amplification effect exploited in many WMbased experiments^{6,26,27,28,29,30,31} is actually limited to a certain range of weak values, determined by the parameter to be evaluated, i.e. the interaction intensity g, and indeed these results were used for choosing the settings of refs^{22,24,36}. Outside of such interval, the weak value approximation can no longer be considered valid, forbidding any accurate weak value measurement and, as a consequence, leading to an unfaithful g extraction due to biased signal amplification.
In the end, we experimentally investigated the limits of WMs, observing how, even in the weak interaction regime, the value of g determines the range of weak values that one is able to extract, putting a threshold to the signal amplification effect^{6,26,27,28,29,30,31} typical of WMs. From our data it results evident that even a very weak coupling, satisfying the constraint \({g}^{2}\ll 1\), could lead to a bias in the weak value measurement in the case of strongly anomalous values. This means that, to determine an unknown weak coupling intensity exploiting the signal amplification mentioned before, we have to be sure not to cross the borders of the first order solution of Eq. (2). Supposing of not having any “a priori” information on g, the only robust strategy to do so is to perform a wide range of measurements for different weak values until the same picture reported in Figs 2 and 3 appears, and then pick only the values belonging to the weak approximation region.
Giving a deeper insight on weak value measurements and their properties, our results pave the way to their widespread diffusion in several applicative fields, e.g. quantum metrology, quantumenhanced measurement and related quantum technologies.
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Acknowledgements
This work has been supported by EMPIR14IND05 “MIQC2” and EMPIR17FUN01 “Become” (the EMPIR initiative is cofunded by the EU H2020 and the EMPIR Participating States) and the MIUR Progetto Premiale 2014 “QSecGroundSpace”. We thank Dr. Mattia P. Levi for contributing to the experimental setup implementation and data analysis.
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I.P.D., M. Gram and M. Gen (responsible of the laboratories) planned the experiment. The experimental realization was achieved (supervised by I.P.D., G.B., M. Gram and M. Gen) by F.P. (leading role) and A.A. The camera was developed and optimized for this experiment by R.L., F.V., A.T. The manuscript was prepared with inputs by all the authors. They also had a fruitful systematic discussion on the progress of the work.
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Piacentini, F., Avella, A., Gramegna, M. et al. Investigating the Effects of the Interaction Intensity in a Weak Measurement. Sci Rep 8, 6959 (2018). https://doi.org/10.1038/s41598018251567
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