Quantum dots (QDs) in III–V semiconductors form excellent sources of indistinguishable single-photons. These emitters have a combination of metrics (brightness, purity, coherence, repetition rate) which no other source can match1,2,3,4. These excellent photonic properties can be extended by trapping a single electron to the QD, enabling spin-photon entanglement5 and high-rate remote spin-spin entanglement creation6. Underpinning these developments are, first, a self-assembly process to create nano-scale QDs; and second, a smart heterostructure design along with high-quality material. The established platform consists of InGaAs QDs embedded in GaAs. However, the InGaAs QDs emit at wavelengths between 900 and 1200 nm, a spectral regime lying inconveniently between the telecom wavelengths (1300 nm and 1550 nm) and the wavelength where silicon detectors have a high efficiency7 (600–800 nm). It is important in the development of QD quantum photonics to extend the wavelength range towards both, shorter and longer wavelengths.

GaAs QDs in an AlGaAs matrix can be self-assembled by local droplet etching8,9 and have a spectrally narrow ensemble10,11. They emit at wavelengths between 700 and 800 nm. This is an important band: it coincides with the peak quantum efficiency of silicon detectors; it contains the rubidium D1 and D2 wavelengths (795 nm and 780 nm, respectively) offering a powerful route to combining QD photons with a rubidium-based quantum memory12. Furthermore, GaAs QDs have typically more symmetric shapes, facilitating the creation of polarisation-entangled photon pairs from the biexciton cascade4,13.

GaAs QDs have also very low levels of strain9,14,15,16,17. In contrast, the high level of strain in InGaAs QDs complicates the interaction of an electron spin with the nuclear spins on account of the atomic site-specific quadrupolar interaction14,18. For electrostatically defined GaAs QDs, the spin-dephasing time, \({T}_{2}^{* }\), has been prolonged to the micro-second regime by narrowing the nuclear spin distribution together with real-time Hamiltonian estimation19. Applied to a droplet GaAs QD, such techniques could prolong the spin dephasing time to values several orders of magnitude above the radiative lifetime. In this case, in combination with optical cavities20, droplet GaAs QDs can potentially serve as fast, high-fidelity sources of spin-photon pairs and cluster states21.

The development of GaAs QDs for quantum photonics lags far behind the InGaAs QDs. Recurrent problems are blinking22,23 (telegraph noise in the emission) and optical linewidths well above the transform limit13,16,23,24,25. Both of these problems are caused by charge noise. On short time-scales, the charge environment is static such that successively emitted photons exhibit a high degree of coherence4,25. On longer time-scales, however, the charge noise introduces via blinking an unacceptable stochastic character to the photon stream. An additional weak non-resonant laser provides control over the noise to a certain extend, though it does not remove the blinking completely22.

For InGaAs QDs, embedding the QDs in an n-i-p diode has profound advantages: the charge state is locked by Coulomb blockade26,27,28; the charge noise is reduced significantly29; and the exact transition frequency can be tuned in-situ via a gate voltage3,30. Such a structure is missing for GaAs QDs13,16,22,23,24,25—in previous attempts, charge-stability was not demonstrated31,32. A materials issue must be addressed: the barrier material AlGaAs must be doped, yet silicon-doped AlGaAs contains DX-centres33,34 which both reduce the electron concentration, causing the material to freeze out at low temperatures, and lead to complicated behaviour under illumination. Here, we resolve this issue—all doped AlGaAs layers have a low Al-concentration. In this case, the DX level lies above the conduction band minimum and thus is unoccupied at cryogenic temperatures33. The QDs are grown in a region with higher Al-concentration, which is well-established for the growth of these QDs8. On GaAs QDs in this device we demonstrate charge-control via Coulomb blockade, optical linewidths just marginally above the transform limit, blinking-free single-photon emission, electron spin initialisation, and a spin-relaxation time as large as  ~50 μs.


Sample design and characterisation

The sample is grown on a GaAs-substrate with (001)-orientation. Below the active region of the sample, a distributed Bragg reflector is grown to enhance the collection efficiency of the photons emitted by the QDs. The QDs are embedded in an n-i-p-diode structure where the QDs are tunnel-coupled to the n-type layer. The n-type back gate consists of silicon-doped Al0.15Ga0.85As. The low Al-concentration in this layer is crucial to avoid the occupation of DX-centres in n-type AlGaAs33,34. A tunnel barrier consisting of 20 nm Al0.15Ga0.85As followed by 10 nm Al0.33Ga0.67As separates the QDs from the n-type back gate. The QDs are grown in the Al0.33Ga0.67As-layer by using local droplet-etching8. The QD-density is nQD = 0.37 ± 0.01 μm−2. Above the QDs, there is 274 nm of Al0.33Ga0.67As followed by a p-type top gate. The top gate is composed of carbon-doped Al0.15Ga0.85As, where reduced Al-concentration is used as well. A schematic bandstructure of the diode is shown in Fig. 1a; all Al-concentrations in this design are small enough that processing into micropillars35 and nanostructures will not be hindered by oxidation36. In Table 1, the design of the full heterostructure is given.

Fig. 1: Tuning the charge state of single GaAs quantum dots.
figure 1

a Schematic band structure (conduction band) of the diode hosting charge-tunable GaAs quantum dots. b The photoluminescence emitted by an exemplary single quantum dot as a function of the gate voltage, Vg. (Positive gate voltage indicates a forward bias.) The corresponding electric field, F, is plotted as an additional x-axis on top. The photoluminescence is resolved in energy by a spectrometer and measured on a CCD-camera. The emission spectrum shows several plateaus corresponding to different charge states of the quantum dot. We observe narrow photoluminescence-linewidths on highly charged excitons where up to eight additional electrons occupy the quantum dot. c Resonance fluorescence from X1+, X0, and X1− charge plateaus measured on another quantum dot (QD1). X1+, X0, and X1− represent the positive trion, the neutral exciton, and the negative trion, respectively. The measurement is performed by sweeping the gate voltage for different laser frequencies. The resonance fluorescence intensity is measured with a superconducting nanowire single-photon detector. This measurement is performed by resonant continuous-wave excitation below saturation. In saturation, the maximum count rate is 6.5 MHz (see Supplementary Fig. 1 for the power saturation curve).

Table 1 Sample design with relevant growth parameters.

We characterise our device by measuring the photoluminescence from a single QD as a function of the gate voltage, Vg, applied to the diode (Fig. 1b). As a function of Vg, the emission lines show a pronounced Stark-shift. At specific gate voltages, discrete jumps in the emission spectrum take place: one emission line abruptly becomes weaker and another line appears. This effect is the characteristic signature of charge-control of a QD via Coulomb blockade26: the net-charge of the QD increases one by one and the emission energy is shifted due to the additional Coulomb interaction with the new carrier.

We fit the relation E = E0 + αF + βF2 to the dependence of the emission energy, E, on electric field, F (Supplementary Fig. 2). The energy jumps between different charge plateaus are removed for the fit. We find α/e = 0.21 nm, the permanent dipole moment in the growth direction, and β = −1.35 × 10−6 eV(kV/cm)−2, the polarisability of the QD37. Extrapolating the fit shows that the Stark shift is zero at a non-zero electric field (F = 7.8 kVcm−1). The non-zero value of α represents a small displacement between the “centre-of-mass” of the electron and the hole wavefunctions. The hole wavefunction is slightly closer to the back gate than the electron wavefunction.

Resonance fluorescence from GaAs QDs

We identify the neutral exciton, X0, from its characteristic fine-structure splitting, as well as a quantum-beat in time-resolved resonance fluorescence (Supplementary Fig. 3). For our device, the fine-structure splittings are distributed over a range of 1–3 GHz (see Supplementary Fig. 4c). The fine-structure splittings are comparable to literature values on (001)-oriented samples4,8. Smaller fine-structure splittings can be obtained by using (111)-oriented samples13 and strain-tuning38. We identify the other charge-states by counting the number of jumps in the emission spectrum as the gate-voltage increases/decreases. We measure emission from highly charged excitons ranging from the two-times positively charged exciton, X2+, to the eight-times negatively charged exciton, X8−. Such a wide range of charge tuning was not previously achieved with any QDs emitting in the close-to-visible wavelengths. Our GaAs QDs give a large range of charge tuning due to their relatively large size8 in comparison to the widely used InGaAs QDs39.

We turn to resonant excitation. This excitation scheme is key for creating low-noise photons and represents a true test of the fidelity of the device as, unlike photoluminescence, continuum states are not deliberately occupied. By sweeping both the gate voltage and excitation laser frequency, we map out three charge plateaus of a single quantum dot (QD1) – X1+, X0, and X1− (see Supplementary Fig. 5 for photoluminescence of QD1). As is visible in Fig. 1c, the exact transition energy of all three charge states can be tuned via Vg across a range of above 1 meV. At a fixed gate voltage, we determine a resonance fluorescence linewidth of X1− to be 0.64 ± 0.01 GHz (full width at half maximum) on scanning a narrow-bandwidth laser over the trion resonance (see Fig. 2a). (resonance fluorescence laser scans on X1+ and X0 are shown in Supplementary Fig. 3). This measurement takes several minutes: the linewidth probes the sum of all noise sources over an enormous frequency bandwidth40. The measured linewidth is very close to the lifetime-limit of Γr/2π = 0.59 ± 0.01 GHz. (It is assumed here the decay is radiative. The radiative decay rate Γr is determined by recording a decay curve following pulsed resonant excitation, Fig. 2b). This result shows that there is extremely little linewidth broadening due to noise in our device. These excellent results are not limited to one individual QD. Shown in Fig. 2d is a linewidth measurement on a second QD (QD2). In the central part of the X1− charge-plateau (from Vg = −0.5 V to Vg = −0.4 V in Fig. 2c), we also measure a close-to lifetime-limited linewidth. On average, the ratio between the measured linewidth and the lifetime limit is 1.08 for QD2. At the edges of the charge-plateau, the linewidth increases—a well-know effect due to a co-tunnelling interaction with the Fermi-reservoir41. Comparably good properties are found for in total seven out of ten randomly chosen QDs with X1− below 785 nm (see Supplementary Fig. 4a, b).

Fig. 2: Time-resolved lifetime and photon-correlation measurements.
figure 2

a Resonance fluorescence linewidth measured on the singly-charged exciton, X1− (QD1). The measurement is performed by sweeping a narrow-bandwidth laser over the X1− resonance. The overall time for the shown scan is  ~8 min. A Lorentzian function (red line) fits perfectly to the data (blue dots), showing an optical linewidth of 0.64 ± 0.01 GHz. b Lifetime measurement on X1− under pulsed resonant excitation. The gate voltage is the same as in a. The measured decay rate (Γr = 3.71 ± 0.04 GHz, corresponding to a lifetime of 1/Γr = 270 ± 3 ps) implies a lifetime-limited linewidth of Γr/2π = 0.59 ± 0.01 GHz (Exponential fit). c Resonance fluorescence of X1− (QD2) as a function of the gate voltage. d Resonance fluorescence linewidth along with the lifetime-limit (obtained from separate lifetime measurements at the corresponding gate voltages). Similar to QD1, the linewidth of QD2 stays very close to the lifetime limit in the plateau centre. e Auto-correlation (g(2)) measured under resonant π-pulse excitation. f Auto-correlation of the resonance fluorescence measured under weak continuous-wave excitation shown on a short time-scale. The g(2)-measurement is normalised44 by dividing the number of coincidences by its expectation value T tbin x1 x2, where T is the overall integration time, tbin is the binning time, and x1, x2 are the count-rates on the two single-photon detectors. g The same auto-correlation measurement as in f but evaluated on a much longer time-scale (milliseconds). The perfectly flat g(2) reveals the absence of blinking.

A remarkable feature is that the close-to-transform limited linewidths are observed despite the large dc Stark shifts of these QDs. Within the X1− plateau of QD1 (Fig. 1c), the dc Stark shift is 0.0347 GHz per V cm−1, about a factor of four larger than the typical dc Stark shifts of InGaAs QDs40. The sensitivity of the transition frequency to the electric field renders the QD linewidth susceptible to charge noise. The close-to-transform limited linewidths reflect therefore an extremely low level of charge noise in the device. Assuming that the slight increase in broadening with respect to the transform limit arises solely from charge noise, the linewidth measurement places an upper bound of  ~3.0 Vcm−1 for the root-mean-square (rms) electric field noise at the location of QD1. This upper bound is comparable to the best gated InGaAs QD devices20,29,40,42,43.

For applications as single-photon source, it is crucial to demonstrate that the photons are emitted one by one, i.e., photon anti-bunching. Therefore, we continue our analysis by performing an intensity auto-correlation of the resonance fluorescence. This g(2)-measurement is shown in Fig. 2e and Supplementary Fig. 6c, d for resonant π-pulse excitation with 76 MHz repetition rate. We observe a strong anti-bunching at zero time delay (g(2)(0) = 0.019 ± 0.008), corresponding to a single-photon purity of 1 − g(2)(0) ~98%. The corresponding measurement under weak continuous-wave excitation is shown in Fig. 2f. (g(2)-measurements versus excitation power, as well as laser detuning are mapped out in Supplementary Fig. 7, where clear Rabi oscillations are shown. In both cases, we find excellent agreement between the measured g(2) and a calculation based on a two-level model.) Also here, we observe a strong anti-bunching proving the single-photon nature of the emission.

Previous resonance fluorescence on GaAs QDs has suffered from blinking, i.e., telegraph noise in the emission22. This is a deleterious consequence of charge noise: either the QD charges abruptly or the charge state of a nearby trap changes, detuning the QD from the excitation laser in both cases. Blinking gives rise to a characteristic bunching (g(2) > 1) in the auto-correction even for driving powers well below saturation22. We investigate this point here. Even out to long (millisecond) time-scales, the g(2)-measurement is absolutely flat and close to one (see Fig. 2g). (We note that our analysis includes a mathematically justified normalisation of the g(2)-measurement44). This result demonstrates that blinking is absent. This is a consequence both of the diode-structure, in particular Coulomb blockade which locks the QD charge, and the low charge noise in the material surrounding the QD.

We subsequently carried out g(2)-measurements with either a small magnetic field along the growth direction or a laser slightly detuned from the QD resonance. In the former case the sensitivity to spin noise is enhanced, while in the latter case the sensitivity to charge noise is enhanced40. In Supplementary Fig. 8, we compare the g(2)-measurements on millisecond time-scales. For the measurement with an additional magnetic field (Supplementary Fig. 8c, d), the g(2) remains flat and stays close to one. In contrast, we observe a small blinking when the laser is detuned (Supplementary Fig. 8e, f). We infer from these results that in our device charge noise is most likely to be responsible for the residual linewidth broadening.

High-fidelity spin initialisation

The diode structure allows us to load a QD with a single electron. The spin of the electron is a valuable quantum resource. To probe the electron-spin dynamics, we probe the X1− resonance fluorescence in a magnetic field (Faraday-geometry). In this configuration, the ground state is split by the electron Zeeman energy, and the excited state is split by the hole Zeeman energy (see Fig. 3a). As the diagonal transitions in this level-scheme are close to forbidden, the X1−-charge-plateau splits into two lines which are separated by the sum of electron and hole Zeeman energies (see Fig. 3b). We find that the X1− charge-plateau becomes optically dim in its centre. This is the characteristic feature of spin-initialisation via optical pumping27,43,45,46. On driving e.g., the \(\left|\uparrow \right\rangle -\left|\uparrow \downarrow \Uparrow \right\rangle\) transition, the trion will most likely decay back to the \(\left|\uparrow \right\rangle\)-state via the dipole-allowed vertical transition. However, due to the heavy-hole light-hole mixing or a weak in-plane nuclear field, it can also decay to the \(\left|\downarrow \right\rangle\)-state through the “forbidden” transtion with a small probability. When the QD is in the \(\left|\downarrow \right\rangle\)-state, the driving laser is off-resonance on account of the electron Zeeman energy. Therefore, the centre of the X1−-charge-plateau becomes dark and the initialisation of the electron spin in the \(\left|\downarrow \right\rangle\)-state is heralded by the disappearing resonance fluorescence. At the plateau-edges, resonance fluorescence reappears due to fast spin-randomisation via co-tunnelling41. By comparing the remaining intensity in the charge-plateau centre to the plateau edges27, we estimate the spin initialisation fidelity to be F = 98.3 ± 0.3%. To confirm that the signal disappears in the plateau-centre on account of optical spin initialisation and not some other process, we perform a measurement with a second laser at a fixed frequency. When the fixed laser is resonant with \(\left|\uparrow \right\rangle -\left|\uparrow \downarrow \Uparrow \right\rangle\) transition, we observe a recovery of the signal (Fig. 3c) on either driving the weak diagonal transition \(\left|\downarrow \right\rangle - \left|\uparrow \downarrow \Uparrow \right\rangle\) or the strong vertical transitions \(\left|\downarrow \right\rangle -\left|\uparrow \downarrow \Downarrow \right\rangle\) with the scan laser. While the fixed laser is tuned to \(\left|\downarrow \right\rangle -\left|\uparrow \downarrow \Uparrow \right\rangle\) transition (at a different Vg), another recovery spot is seen as the scan laser drives the vertical transition \(\left|\uparrow \right\rangle -\left|\uparrow \downarrow \Uparrow \right\rangle\). This confirms the optical spin-initialisation mechanism27,45. From the energy splitting at the plateau edges, we determine the electron and hole g-factors17, ge = −0.076 ± 0.001 and gh = 1.309 ± 0.001. For the positively charged trion (X1+), we also observe high-fidelity optical spin-initialisation (Supplementary Fig. 9) and narrow linewidths (0.62 GHz, see Supplementary Fig. 3), in this case of a hole spin.

Fig. 3: Initialisation of a single electron spin.
figure 3

a Level scheme of the negative trion X1− in a magnetic field (Faraday geometry). b Optical spin-initialisation via optical pumping on X1−. The measurement is carried out at B = 6.6 T. In the plateau centre, the resonance fluorescence disappears due to successful spin-initialisation; at the plateau edges it remains bright due to rapid spin-randomisation via co-tunnelling41. c Optical spin-initialisation and re-pumping with a second laser at a fixed frequency (laser 2). Recoveries of the signal are found in the plateau centre. d Schematic of the time-resolved spin-pumping measurement. e Resonance fluorescence intensity as a function of time. The signal drops due to optical spin-initialisation after turning the driving laser on. The overall intensity is larger when the time-delay τoff between the laser pulses is larger. In this case, the electron spin has more time to relax back from the off-resonant state. f Resonance fluorescence intensity as a function of the waiting time between the spin-pumping laser pulses. The magenta line is an exponential fit to the data (blue dots). From this measurement we extract an electron-spin lifetime of T1 ~ 48 ± 5 μs.

How long-lived is the prepared spin state? To answer this question, we measure the time-dependence of the X1− spin initialisation43,46. The scheme is illustrated in Fig. 3d. First, we drive the \(\left|\uparrow \right\rangle -\left|\uparrow \downarrow \Uparrow \right\rangle\) transition for τon = 3 μs. During this laser pulse, the signal decreases due to optical spin-initialisation (Fig. 3e). Subsequently, we turn the laser off for a time τoff, and then turn the laser back on again. During the off-time the electron spin randomises. Fig. 3e shows that the resonance fluorescence signal is stronger when the waiting time τoff is longer. The reason for this effect is that with increasing τoff the spin has more time to randomise. For a short value of τoff, in contrast, the spin remains in the off-resonant state—it has no time to relax before the next optical pulse is applied. By measuring the signal strength for varying τoff (Fig. 3f), we determine an electron-spin relaxation time of T1 = 48 ± 5 μs. Our result shows that the design of the tunnel-barrier between QDs and back gate is well suited for spin-experiments on single QDs. This T1 value is significantly larger compared to the GaAs QDs without the n-i-p-diode structure23. The point is that the T1 time is potentially longer than the coherence time T2, such that the relaxation process governing T1 is unlikely to limit the coherence time T247.


In summary, we have developed charge-tunable GaAs QDs with ultra-low charge noise. We show notable improvements of the GaAs QDs properties: optical linewidths are close-to lifetime-limited, blinking is eliminated, and long electron-spin lifetimes are achieved. From a materials perspective, the crucial advance is the new diode structure hosting GaAs QDs—a key feature is that all the doping is incorporated in layers of low Al-concentration. In this way, the occupation of DX-centres is avoided and the AlGaAs layers are conducting at low temperatures. The concepts developed in this work can be transferred to thinner diode-structures that allow integration into photonic-crystals and other nanophotonic devices3,36. From a quantum photonics perspective, our results pave the way to bright sources of low-noise single photons close to the red part of the visible spectrum. This will facilitate the developments of both short-range networks and a hybrid QD-rubidium quantum memory. On account of the low-strain environment in GaAs QDs, our work can also open the door to prolonged electron spin coherence.


Sample fabrication

The sample heterostructure and the quantum dots are grown by molecular beam epitaxy (MBE). The MBE setup is similar to the one described in ref. 48. The complete heterostructure of the sample is shown in Table 1. All doped layers in AlGaAs have low Al-concentration (<20%). The quantum dots are surrounded by AlGaAs with higher Al-concentration (33%), to enable the growth of QDs close to rubidium-frequencies and with small fine-structure splittings8,11. We fabricate separate Ohmic contacts to the n+ and p++ layers. For the n-type back gate, the sample is locally etched down by  ~360 nm in a mixture of sulfuric acid and hydrogen peroxide (concentrated H2SO4: 30% H2O2: H2O = 1: 1: 50). NiAuGe is then deposited by electron-beam evaporation (with three steps: 60 nm AuGe (mass ratio 88:12), 10 nm Ni, and 60 nm AuGe), followed by thermal annealing at  370 C for 60 s and 420 C for 30 s. For the p-type top gate, a thin contact pad consisting of Ti (3 nm)/Au (7 nm) is evaporated locally on the top surface of the sample. Both contacts are electrically connected with silver paint.

Experimental setups

The sample is cooled down to 4.2 K in a liquid helium cryostat. We perform photoluminescence with a 632.8 nm He–Ne laser. The photoluminescence is collected by an aspheric objective lens (numerical aperture NA = 0.71) and sent to a spectrometer. Resonance fluorescence is performed with a narrow-band laser (1 MHz linewidth), using a cross-polarisation confocal dark-field microscope22,49 to distinguish QD-signal from the scattered laser light. It is detected using superconducting-nanowire single-photon detectors and a counting hardware with a total timing jitter of 35 ps (full width at half maximum).

Statistics of QD linewidths

In our device, GaAs QDs with a small height (emission wavelength below  ~785 nm) tend to have excellent optical properties. We find that more than every second QD has a close to lifetime-limited linewidth (see Supplementary Fig. 4a,b). This includes QDs close to the 87Rb D2 line (~780 nm). For QDs larger in size (emission wavelength above  ~785 nm), the QD linewidths are usually broader. The reason is probably the following: the GaAs QDs in our sample are grown by infilling nano-holes droplet-etched into a 10 nm-thin layer of Al0.33Ga0.67As (see Table 1). The depths of the nano-holes, and therefore the heights of the QDs, typically range from 5 nm to 10 nm8,11. A QD emitting at higher wavelength tends to have a larger height11. When the height of a QD comes close to 10 nm, the optical properties could be affected by the Al0.33Ga0.67As/Al0.15Ga0.85As interface. A simple solution is to make the Al0.33Ga0.67As-layer 5 nm thicker. In this case, we expect good optical properties also for QDs of higher wavelengths.

Auto-correlation under different excitation schemes

We investigate the stability of the QD under different excitation schemes. We start with continuous-wave (CW) excitation. We perform auto-correlation measurements on X1− at a constant gate voltage while exciting the QD with (i) an above-band laser (λ = 632.8 nm), (ii) a laser resonant with the p-shell, and (iii) a laser resonant with the s-to-s transition. The results are shown in (i) Supplementary Fig. 6a, (ii) Supplementary Fig. 6b, and (iii) Fig. 2g, respectively. In all three cases, the g(2) stays very flat and close to one—there is no blinking even on a long time-scale. This shows that the QD is a very stable quantum emitter under all three CW excitation schemes. From an applications point of view, it is usually necessary to drive the QD with a resonant pulsed laser. We investigate the auto-correlation under resonant π-pulse excitation in Fig. 2e. An evaluation of this g(2)-measurement on a longer time-scale is plotted in Supplementary Fig. 6c, where the y-axis is displayed on a logarithmic scale to resolve the central peak. To investigate whether a strong π-pulse introduces any blinking, we plot the g(2)-measurement in a histogram plot (Supplementary Fig. 6d) by summing up the coincidence events for every single pulse. This sum is divided by the expectation value for a perfectly stable source: the normalisation factor is x1x2Tint/frep, where frep is the repetition rate of the pulsed laser, x1, x2 represent the count rates of the two detectors used for a Tint-long g(2)-measurement. A derivation of the normalisation factor is given in Supplementary Fig. 6. Importantly, the histogram bars at non-zero time delay are flat and very close to one; the bar at zero delay is close to zero. This shows that the QD is a stable single-photon emitter for resonant π-pulse excitation.

Potential noise source affecting the QD-linewidth

The g(2)-measurement shown in Fig. 2f,g is performed on a trion at zero magnetic field when the CW laser drives the QD resonantly. The sensitivity can be enhanced towards either spin noise or charge noise by applying a small magnetic field along the growth direction, and detuning the laser slightly from the QD-resonance by δ, respectively. A trion state is degenerate at zero magnetic field, consisting of two opposite spin ground states. When applying a magnetic field B, the degeneracy is lifted and the trion state is split into two by a Zeeman energy Ez = gμBB, with g being the electron or hole g-factor, and μB the Bohr magneton. We maximise the spin noise sensitivity by applying a small magnetic field such that \({E}_{z}=\frac{\tilde{\Gamma }}{\sqrt{3}}\) (Supplementary Fig. 8c). Here \(\tilde{\Gamma }\) represents the full width at half maximum (FWHM) of the QD emission. For the maximised spin noise sensitivity, the g(2)-measurement does not show any clear sign of bunching (Supplementary Fig. 8d). The charge noise sensitivity is maximised when the laser is detuned from the QD by \(\delta =\frac{\tilde{\Gamma }}{2\sqrt{3}}\) (Supplementary Fig. 8e). In this configuration, we observe a small bunching peak in the g(2)-measurement (Supplementary Fig. 8f). This result suggests that charge noise on a millisecond time-scale is responsible for the slight linewidth broadening.