Abstract
The ability to read out the state of a single confined spin lies at the heart of solid-state quantum-information processing1. Although spin measurements using Faraday rotation of light polarization have been implemented in semiconductor spin ensembles2,3,4, single-spin read-out has only been achieved using transport measurements5,6. Here, we demonstrate an all-optical dispersive measurement of the time-averaged spin state of a single electron in a quantum dot. We obtain information on the spin state through conditional Faraday rotation of a spectrally detuned laser, induced by the polarization- and spin-selective trion (charged quantum dot) transitions. To assess the sensitivity of the technique, we use an independent resonant laser for spin-state preparation7. We infer that there are ∼10 spin-flip Raman scattering events (that is, back-action) within our measurement timescale. Straightforward improvements such as incorporating solid-immersion lenses8,9 and higher efficiency detectors should allow for back-action-evading spin measurements, without the need for a cavity.
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Main
Absorption and dispersion coexist in an optical field’s response to a spectrally detuned optical transition. Although these responses are of comparable strength for small detunings, dispersive response dominates over the absorptive part as the detuning is increased. Measurement of the dispersive response provides information about the ground (spin) state, if the transition obeys spin-selective optical selection rules, as is the case for a quantum dot (QD) confining a single excess electron7,10. Here, we demonstrate measurement of a QD spin by detecting this dispersive response through Faraday rotation (FR) of a far-detuned linearly polarized laser.
Theoretical proposals on the basis of FR from a microcavity-embedded QD have suggested that quantum non-demolition11 measurement of a single spin could be implemented12,13. Remarkably, our observations suggest that the back-action-evading spin measurement in the basis defined by the Pauli operator σz (the strong confinement axis) could be realized even in the absence of an optical cavity enhancing the FR. We estimate that the QD scatters a photon every 2 μs; the role of these events is to leak state information into the field reservoir, thus, inducing back-action on the σx observable and collapsing the state into a σz eigenstate. The spin-flip Raman scattering events, which lead to back-action on the measured observable (σz), occur once every 2 to 20 ms. Although it is impossible to avoid Rayleigh scattering within a measurement time yielding a signal-to-noise ratio exceeding unity, spin-flip scattering can be negligible if the ratio of the peak absorption cross-section and the laser area (σQD/AL) considerably exceeds the ratio of the Rayleigh and spin-flip Raman scattering rates (that is, the branching ratio into the spin-flip scattering channel)7. We have determined that the branching ratio in self-assembled QDs is between 10−3 and 10−4 and is primarily due to hyperfine-induced state mixing.
Spin measurements could also be carried out using resonance fluorescence or absorption experiments. However, owing to background Rayleigh scattering and limited collection efficiency, the timescales needed to measure the spin state via the resonance fluorescence technique exceed the spin-flip timescales. Resonant absorption measurements are likewise limited by electrical noise that dominates over the shot noise for laser intensities that do not saturate the QD transitions. FR, however, allows for shot-noise-limited spin measurements with the highest signal-to-noise ratio among these techniques, by a proper choice of laser intensity and detuning. Furthermore, for QDs embedded in cavities, FR provides the only measurement scheme that can avoid light scattering completely; this is crucial in measurement-induced-entanglement schemes or in systems with a considerable branching ratio into the spin-flip scattering channel.
A single electron confined in a QD presents a four-level system in the trion representation, as illustrated in Fig. 1a. The ground state consists of an electron in the |↓〉(|↑〉) state. The excited state corresponds to the QD with two electrons forming a singlet and a hole with angular momentum projection Jz=−3/2(3/2) along the growth direction. The trion transition, , is allowed only for [σ(−)] ([σ(+)]) circular polarization as determined by the optical selection rules. If a linearly polarized laser—for example, [π(+)]—feels this transition, the [σ(−)] ([σ(+)]) polarization component acquires a phase shift rotating the laser’s polarization by an angle θ (−θ) in the linear basis. Owing to Pauli blockade14, only one of these transitions is available at any given time and the laser polarization is rotated in the positive or negative angular direction depending on the electron’s spin state. In our experiments, we exploit precisely this spin-state-dependence of the laser polarization.
Figure 1b shows our detection scheme. A polarized laser propagates through a gated heterostructure incorporating QDs. A polarizing beam splitter distributes the transmitted light into two linear polarizations in the rectilinear basis of (X, Y) and directs each arm to a photodiode. Along with each detector’s output (Tx and Ty), such a configuration allows us to measure their sum and difference simultaneously. The sum (Tsum) normalized to the total incident laser intensity indicates a change of photon number in the total light, yielding the absorptive response, whereas the (normalized) difference of the two signals (Tdiff) is linked to the polarization rotation arising from the dispersive response.
In the absence of an external magnetic field, the trion transition has a twofold spin degeneracy. Therefore, although we fully observe the absorptive response in the summed detector signals, the dispersive response is exactly cancelled owing to the fast spin-flips induced by the hyperfine interaction15. Under an external magnetic field however, the Zeeman splitting (EZeeman) lifts the spectral degeneracy of the two spin-selective trionic transitions (as in Fig. 1a). Consequently, the dispersive response is expected to appear along with the absorptive part in the spectral vicinity (Δ≪EZeeman) of one of the Zeeman-split transitions in the form
where α0 is proportional to the ratio σQD/AL and incorporates heterostructure-induced mode mismatch, γ is the total linewidth measured in absorption measurements, Δ is the spectral detuning of the probe laser and θ is the FR angle.
Figure 1c shows how the sum (black circles) and difference (red circles) signals from one of the Zeeman-split transitions behave as a function of laser detuning for two different polarizations, when an external magnetic field of 1 T is applied along the strong confinement axis of the QD. The transitions are split by 26 GHz, which is ∼60 times larger than the total transition linewidth γ, and the laser’s response in the near vicinity of the [σ(−)]-polarized transition linked to the spin-down electronic state is shown. When the laser is also circularly polarized (left plot), it acquires an overall phase that cannot be detected leading to a purely absorptive signal (black circles). The same scan with a linearly polarized laser (right plot) shows the dispersive response (red circles) alongside the absorptive response (black circles): as the acquired phase is now relative, it leads to a linear polarization rotation. The solid grey lines are fits using equation (1) for the dispersive QD response. Both curves in the [π+] case have α0=0.14%,ΩL2=γ2/2 and γ=2π×466 MHz, as obtained from line-broadening in saturation spectroscopy, where full-width at half-maximum =2×{(γ/2)2+ΩL2/2}1/2. At such small detuning with respect to Zeeman splitting, the laser experiences FR primarily due to one Zeeman transition nearby. The data presented here are obtained in the cotunnelling regime to avoid spin pumping7. We note here that similar dispersive response signatures of single QDs have recently been reported16. In contrast to the work presented here, the dispersive signals observed there16 are polarization and spin independent and arise from an interference effect that depends on the QD position with respect to the laser focal spot in a planar Fabry–Perot cavity.
We now consider probe-laser detunings that are larger than Zeeman splitting (Δ>EZeeman), where the difference signal arises from a competition between the two transitions. Figure 2a (top) shows the difference signal when the probe laser is blue-detuned by 20 to 40 GHz with respect to the [σ(+)]-polarized transition obtained in a 60 s measurement timescale per point. The black circles show the difference (offset) signal when the preparation laser is left detuned from the two Zeeman transitions: in this case, no state preparation is implemented and the electron spin state is effectively thermalized being close to a completely mixed state, as spin-flip events occur on timescales shorter than our measurement timescale. As the gate voltage is increased, the Zeeman-split optical transitions experience an equal strength of d.c.-Stark shift. Consequently, the detuning of the probe laser with respect to the two transitions is also decreased, creating an offset signal in accordance with the incommensurate detunings and partial cancellation of the FRs.
The red circles show the difference signal when the frequency of the weak preparation laser is in the near vicinity of the [σ(−)]-polarized Zeeman transition. At a gate voltage of 415 mV, the preparation laser hits resonance and the electron is spin cooled to the spin-up state with near-unity fidelity due to state-mixing-induced spin-flip Raman transitions7. Therefore, we no longer observe the difference of two dispersive responses, rather the full signal due to one spin-state. Figure 2a (bottom) shows a similar measurement when the preparation laser is tuned to resonance with the [σ(+)]-polarized Zeeman transition again at a gate voltage of 415 mV, preparing the electron in the spin-down state. The full dispersive signal from a single electron spin is recovered, but now with opposite sign, indicating FR in the opposite direction. The amplitude of this signal is less than that of Fig. 2a (top) in accordance with the additional detuning of EZeeman=26 GHz due to Zeeman splitting. Beyond a gate voltage of 450 mV, the QD charging state switches from one excess electron to two electrons, forming a spin-singlet ground state. As the trionic transitions are no longer present beyond this point, the laser experiences no dispersive response. Figure 2b shows the 60 s time-averaged FR angle obtained from the dispersive signal for various probe-laser and preparation-laser detunings. As expected, the FR angle reaches a positive (negative) maximum value when the pure spin-up (spin-down) state is enforced. When the electron spin is left in a thermal mixed state, the value of the FR angle is reduced for probe-laser detunings (56 GHz and 92 GHz) much larger than Zeeman splitting (26 GHz). After submission of this work, we became aware of a similar time-averaged single-spin measurement, where partial spin preparation is achieved via an above-bandgap laser17.
Figure 3a shows a full map of the dispersive signal at a 100 ms measurement timescale per data point, plotted as a function of gate voltage and probe-laser detuning when the preparation laser is [σ(+)]-polarized. The centre frequency of the probe laser is detuned 92 GHz (∼200 times γ) for the top figure and 56 GHz for the bottom figure. Once again, a gate voltage of 415 mV marks the preparation of the spin-down state. Figure 3b shows a similar measurement when the preparation laser is [σ(−)]-polarized to prepare the spin-up state on resonance. As a consequence of Zeeman splitting, the probe laser is detuned 66 GHz for the top figure and 30 GHz for the bottom figure from the nearest transition. The signal from a spin in a mixed state remains identical, whereas the signal from the optically prepared spin switches sign. The middle plot shows line projections of the FR angle at 415 mV for both cases, which are in accordance with the expected inverse detuning (Δ−1) dependence.
Achieving spin read-out that is fast with respect to spin-flip dynamics, that is, T1 time, is only half the story. If, during this measurement, back-action on the measured observable (σz) occurs on a timescale still faster than the natural spin-flip times, then the measured dynamics will be distorted by the back-action. Therefore, although the measurement time can be reduced with technical improvements, it is essential that the probability of a back-action event in the form of spin-flip Raman scattering remains small within the T1 time, that is, Tmeasure<T1<Tback-action. We cannot claim a quantum non-demolition or back-action-evading measurement here, as during the required measurement time to obtain a unity signal-to-noise level (100 ms), between 5 and 50 back-action events occur (for a branching ratio of 10−4 and 10−3, respectively). This limitation arises from the fact that our optical system has a numerical aperture of 0.5 and a photodetector efficiency of 10%; under these conditions, (σQD/AL) cannot safely exceed the branching ratio. By using a combination of solid-immersion lenses matched to the refractive index of GaAs (nGaAs=3.5) and commercially available photodetectors with 80% efficiency, achieving a ∼100-fold improvement of (σQD/AL) is plausible. It would then be possible to effectively eliminate spin-flip Raman scattering from the probe laser within the anticipated measurement time of ∼10 ms. In fact, on the basis of the predicted phonon18,19 and cotunnelling20 limited spin-flip times, we could imagine resolving spin quantum jumps with these improvements. Alternatively, incorporating gated structures into photonic crystal nanocavities21 is demanding, but the existence of a far-detuned cavity mode could well be the way to obviate measurement back-action, at the same time allowing for coherent resonant manipulation of spins.
Methods
Sample structure and apparatus
The self-assembled InAs/GaAs QDs used in this experiment are grown by molecular beam epitaxy. Emission is blue-shifted by the partially covered island technique. The QDs are embedded in a Schottky-type heterostructure to achieve charge tuneability22. The sample composition from the bottom substrate to the top surface is as follows: GaAs substrate \20 nm n-GaAs with 4×1018 cm−3 doping level \35 nm GaAs tunnel barrier \QD layer \12 nm GaAs \50 nm Al0.4Ga0.6As \88 nm GaAs \5 nm titanium window. The bias voltage between the titanium window and the n-GaAs layer determines the electric field across the structure and controls the charging of the QDs.
All measurements are carried out in a liquid helium bath cryostat operating at 4.2 K. The numerical aperture of the confocal microscope system is 0.55, resulting in a diffraction-limited laser spot with a diameter of ∼1 μm. The QD density of the sample is chosen to yield essentially one QD at a time within the focal area and its optical transitions can be identified by their spectral signatures. A magnetic field of up to 10 T in Faraday configuration can be applied using a superconducting magnet. Piezo-electric positioners are used to move the sample in all three dimensions.
Optical measurement techniques
For the initial characterization and identification of the QD optical transitions and charging states, conventional micro-photoluminescence as a function of gate voltage is carried out23. The excitation laser energy is 1.6 eV and the collected photoluminescence signal is sent to a liquid-nitrogen-cooled charge-coupled device (LN2-CCD) through a 0.75-m spectrometer with a 1,500 lines mm−1 diffraction grating. The spectral resolution of this detection system is ∼30 μeV.
Once the two optical transitions of the single-electron-charged QD are identified, a polarization-sensitive differential transmission technique is used. The excitation laser is tuned to the vicinity of the optical frequency of the relevant transition, which in turn can be tuned by gate voltage, and the transmitted laser light on scattering from the QD is detected on the other side of the sample by a linear polarization analyser unit. This detection unit is composed of a polarizing beam splitter separating the linear basis X and Y polarization components of the light and redirecting each to a silicon-based p–i–n diode photodetector, as indicated in Fig. 1b. The spectral resolution of this technique is ∼0.08 μeV (20 MHz) as dictated by gate-voltage noise and laser stability. Owing to the level of low-frequency noise of the system, lock-in detection is used following a 3.34 kHz gate-voltage modulation24. The detection system is laser shot-noise limited for an off-resonant probe-laser power of 2 μW.
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Acknowledgements
This work was supported by NCCR Quantum Photonics. The authors acknowledge many useful discussions with G. Giedke, A. Högele, C. Galland, G. Fernandez, J. Taylor, J. Grond, and G. Salis. M.A. and J.D. would like to thank J. Cash for technical assistance.
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Atatüre, M., Dreiser, ., Badolato, A. et al. Observation of Faraday rotation from a single confined spin. Nature Phys 3, 101–106 (2007). https://doi.org/10.1038/nphys521
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DOI: https://doi.org/10.1038/nphys521
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