Abstract
The optical microresonatorbased frequency comb (microcomb) provides a versatile platform for nonlinear physics studies and has wide applications ranging from metrology to spectroscopy. The deterministic quantum regime is an unexplored aspect of microcombs, in which unconditional entanglements among hundreds of equidistant frequency modes can serve as critical ingredients to scalable universal quantum computing and quantum networking. Here, we demonstrate a deterministic quantum microcomb in a silica microresonator on a silicon chip. 40 continuousvariable quantum modes, in the form of 20 simultaneously twomode squeezed comb pairs, are observed within 1 THz optical span at telecommunication wavelengths. A maximum raw squeezing of 1.6 dB is attained. A highresolution spectroscopy measurement is developed to characterize the frequency equidistance of quantum microcombs. Our demonstration offers the possibility to leverage deterministically generated, frequency multiplexed quantum states and integrated photonics to open up new avenues in fields of spectroscopy, quantum metrology, and scalable, continuousvariablebased quantum information processing.
Introduction
Optical microresonators employ the Kerr nonlinearity^{1} to provide broadband parametric gain through fourwave mixing among cavity resonance modes, where pairs of pump photons can be annihilated to generate signal and idler photons at lower and higher frequencies. The Kerr parametric process has been used to demonstrate microresonatorbased frequency combs (microcombs)^{2,3} and dissipative Kerr cavity solitons^{4,5,6,7}, which have revolutionized a wide range of applications from metrology^{8} to spectroscopy^{9}. The quantum aspects of microcomb have been studied recently^{10,11,12,13,14,15} for its capability of providing hundreds of frequency multiplexed quantum channels from a single microresonator. Access to individual quantum channels is possible through offtheshelf wavelengthdivisionmultiplexing filters thanks to microcombs’ large freespectralranges (FSRs), which range from a few GHz to 1 THz^{16,17} as opposed to the finer FSRs of fiber or bulk resonatorbased combs. When combined with integrated photonic circuits, quantum microcombs have the potential to revolutionize photonic quantum information processing.
So far, experiments of quantum microcombs have been limited to the probabilistic regime^{11,12,13,14}, where entanglement is measured between randomly emitted photon pairs with postselecting, coincidence detection. The photon coincidence rate suffers from exponential decrease with the increase of photon number in a quantum state. Quantum architectures built upon probabilistic quantum states are not scalable without quantum memory, which allows repeatuntilsuccess strategies^{18,19}. In contrast, a quantum microcomb in the deterministic regime, where the entanglement among different frequency modes can be deterministically generated and detected, will be a significant step forward towards the scalable quantum architecture on photonic chips.
One approach to constructing deterministic quantum microcombs is to leverage twomode squeezing and create unconditional entanglement between the optical fields in optical frequency combs^{20,21,22}. Squeezed light^{23}, with quantum uncertainty below than that of the vacuum field, has broad applications in science and technology, ranging from enhancing the gravitational wave detection sensitivity in LIGO^{24}, Gaussian boson sampling^{25,26}, to continuousvariablebased quantum computing (CVQC)^{27,28,29,30}. The unconditional entanglement created by twomode squeezing is between continuous optical fields, which can serve as quantum modes (qumodes) to encode quantum information through continuousvariablebased (CV) approaches^{31} for applications in universal quantum computing^{27,28,30}, unconditional quantum teleportation^{32}, quantum dense coding^{33}, quantum secret sharing^{34}, and quantum key distribution^{35}. Unlike probabilistic photonic qubit approaches, the unconditional entanglement in CV approaches enables the number of entangled quantum modes (qumodes) in a quantum state to be deterministically scaled up through frequency^{20,21,36}, time^{37,38,39}, or spatial multiplexing^{40}, which provides a scalable physical platform for continuousvariable quantum computing^{31}. Squeezing is conventionally generated through nonlinear optics in bulk optical systems, such as optical parametric oscillators (OPOs)^{23,41}, or atomic vapor^{42,43}. Squeezed quantum microcombs, when combined with integrated photonic circuits, Gaussian and nonGaussian measurements, can serve as simple and compact building bricks for CV universal quantum computing^{44}, entanglementassisted spectroscopy^{45}, and quantum networking for distributed quantum sensing^{46}. While the generation^{47,48,49,50,51,52,53,54,55,56} and detection^{57} of one or two squeezed frequency qumodes, and the generation of 8 spatial qumodes^{26} have been shown in miniaturized platforms recently, a squeezed microcomb has not been reported yet.
In this work, we demonstrate a deterministic, twomodesqueezed quantum frequency comb in a silica microresonator on a silicon chip. The Kerr parametric process generates unconditional Einstein–Podolsky–Rosen entanglement, i.e., twomode squeezing, between the optical quadrature fields of the qumode pairs in the microresonator^{10,55}. 40 frequency multiplexed qumodes, in the form of 20 twomode squeezed comb pairs, are measured at telecommunication wavelengths. The twomode squeezing is verified by measuring the noise variance through balanced homodyne detection. The maximum raw squeezing of 1.6 dB and maximum antisqueezing of 6.5 dB are attained. A corresponding 3.1 dB squeezing at the output waveguide can be inferred after correcting system losses. A qumode spectroscopy measurement is developed to characterize the frequencies of qumodes with a resolution of 5 MHz in 1 THz optical span. The frequency equidistance of qumodes can simplify homodyne detection in CV quantum information processing, as a simple laser frequency comb can serve as local oscillators (LOs) for all qumodes. In our experiments, the number of accessible qumodes is limited by the a 1 THz optical span of the LOs. The optical span of a quantum microcomb is ultimately set by the chromatic dispersion of the microresonator, which determines the bandwidth of Kerr parametric gain.
Results
Squeezed quantum microcombs
The microresonator used in this work is a 3 mm diameter silica wedge resonator with 22 GHz FSR on a silicon chip^{58} (Fig. 1). The resonator’s intrinsic quality factor (Q_{o}) is 79 million, and a singlemode tapered fiber is used as the coupling waveguide. The resonator is overcoupled to achieve large field escape efficiency, η = κ_{c}/(κ_{c} + κ_{0}), of 83%, where κ_{0} and κ_{c} are the intracavity dissipation rate and the resonatorwaveguide coupling rate. An amplified continuouswave (cw) laser is used as the pump of the resonator, and its frequency (ω_{p}) is phaselocked to the resonance mode at 1550.5 nm through Pound–Drever–Hall (PDH) locking technique^{59}. The pump power in this experiment is set to 120 mW, which is 0.5 dB below the parametric threshold of 135 mW. The dependence of squeezing on the input pump power is discussed in the Methods section. At the through port of the resonator, a narrowband fiberBragg grating (FBG) filter is used to filter out the pump field and the amplified spontaneous emission (ASE) noise from the erbiumdoped fiber amplifier (EDFA). In principle, the bichromatic LOs for twotone homodyne detection can be derived from a soliton microcomb^{6}. However, in the present measurement, an electrooptic modulation (EOM) frequency comb^{60} is used, where tens of modulation sidebands are created by strong electrooptic phase modulation at modulation frequency f_{m} on the cwlaser. A programmable linebyline waveshaper is then used to select a pair of comb lines as the LOs (see Fig. 2). A periodic ramp voltage is applied on a phase modulator (PM) with V_{π} = 2.3 V to scan the phase of the LOs. The LOs and the resonator pump laser are coherent with each other since they are derived from the same cwlaser, and the electrooptic modulators coherently transfer photons from the pump to the modulation sidebands. A detailed description of the experimental setup is provided in the “Methods” section.
The quadrature noise variances of 20 sets of comb pairs (40 qumodes) are measured by means of balanced homodyne detection. To measure the quadrature noise variance of qumodes (−N, N), the EOM comb modulation frequency f_{m} and the programmable waveshaper are adjusted to precisely match the frequencies of LO pairs to ω_{p} ± N × D_{1}, where N is the relative mode number from the mode being pump (N = 0), and D_{1}/2π = 21.95258 GHz is the FSR of the resonator at 1550.5 nm wavelength. In each measurement, the phase of the LOs is ramped to yield varying quadrature variances. Figure 2b shows a representative quadrature noise variance (blue) relative to the shot noise (red) for qumodes (−4, 4). A 30point moving average is used to smooth out the fluctuations in the noise variance measurement. The raw squeezing of 1.6 ± 0.2 dB and antisqueezing of 5.5 ± 0.1 dB are directly observed, and they are obtained by averaging the displayed extrema. The uncertainty is concluded with a 95% confidence interval under tdistribution. The quadrature noise variances of all 40 qumodes are shown in Fig. 2c, and squeezing/antisqueezing are observed for all 40 qumodes. The number of measurable qumodes is limited by the 1 THz optical span of the EOM comb. All measurements are taken at 2.7 MHz frequency, 100 kHz resolution bandwidth (RBW), and 100 Hz video bandwidth (VBW) on an electrical spectrum analyzer (ESA). The noise levels of qumodes (−1, 1) to (−3, 3) are not presented here as their measurements are affected by the transmitted ASE noise from the EDFA near the pump frequency. This can be addressed in the future by using a filter with bandwidth much smaller than the FSR of the resonator, or by increasing the intrinsic quality factor of the cavity and reducing the parametric oscillation threshold to eliminate the need for the EDFA. Finally, as shown in Fig. 2d, no quantum correlation (twomode squeezing) is observed for uncorrelated comb pairs. This serves as a critical check for our twotone homodyne detection.
The raw squeezing and antisqueezing levels of all 40 qumodes are summarized in Fig. 3a. The raw squeezing in our experiment is primarily limited by the 83% cavity escape efficiency, 1.7 dB optical loss, and ~89% photodiode quantum efficiency. The total efficiency after the tapered fiber is 60%. Our 1.6 ± 0.2 dB raw squeezing is among the highest raw squeezing measured for miniaturized Kerr OPOs^{56}, while the highest squeezing ever achieved is 15 dB in a bulk χ^{(2)} OPO^{61}. 6 dB singlemode squeezing was reported earlier in an integrated waveguide^{53}, which indicates that large squeezing is possible in integrated photonic platforms. Recent theoretical studies have suggested that quantum error correction and faulttolerant quantum computing is possible in photonic CVbased approaches^{30} when squeezing reaches 10 dB^{62}.
The antisqueezing levels near qumodes (−10, 10), and from (−17, 17) to (−23, 23) are observed to be smaller than that of other qumodes. We suspect this is caused by spatialmode interaction between different transverse mode families in the resonator, which not only modifies local dispersion^{63} but provides a path to dissipate optical fields from the squeezegenerating mode to another spatial mode^{64}. The spatialmodeinteraction can be identified by measuring the frequency spectrum of a resonator. The relative mode frequencies of the resonator, Δω_{N} = ω_{N} − ω_{0} − N × D_{1}, are measured with sideband spectroscopy method^{65} and presented in Fig. 3b, where ω_{N} is the resonance frequency of relative mode number N. An avoided mode crossing^{63} was found near mode −8, and resonance frequencies below mode −18 and above mode 19 are observed to change abruptly. These are likely caused by the spatialmode interaction and hybridization between two transverse cavity modes. The mode numbers that are affected by spatialmodeinteraction in the mode spectrum coarsely align with that of the dips in antisqueezing measurement. More systematic studies will be performed in the future to understand the mechanism of how spatialmodeinteraction affects squeezing and antisqueezing. Finally, the impact of spatialmode interaction can be eliminated in the future by using a microresonator with a single transverse mode family^{66,67}.
Squeezed microcomb qumode spectroscopy
A qumode spectroscopy method is developed to characterize the frequency equidistance of squeezed qumodes, a prerequisite of frequency combs. Similar to the classical cavity mode spectrum, we can define the relative qumode spectrum as \({{\Delta }}{\omega }_{N}^{Q}\,=\,{\omega }_{N}^{Q}\,\,{\omega }_{0}\,\,N\,\times\, {D}_{1}\), where \({\omega }_{N}^{Q}\) is the optical frequency center of the Nth qumode. The relative qumode spectrum represents the qumode frequency deviation from equidistance. To identify the relative qumode spectrum, the twosided squeezing/antisqueezing spectral line shape is measured for each pair of qumodes, and the center frequency of the spectral line shape yields the relative qumode frequency. In the measurement, the ±Nth LO frequencies are detuned by ±δ from the equidistant frequencies, ±N × FSR, and noise variances are measured at each detuning point for qumodes (−N, N). For each pair of qumodes, the detuning (δ) is varied from −30 MHz to +30 MHz with an interval of 5 MHz, which sets the resolution of the line shape measurement. Measurements of qumodes (−4, 4) at δ = −20, −10, 0, 10, 20 MHz are shown as examples in Fig. 4b. At each detuning point, squeezing and antisqueezing levels can be extracted by averaging the extrema. We plot the squeezing/antisqueezing levels versus detuning (δ) for all qumodes in Fig. 4c, which manifest the twosided spectral line shape of the qumodes. The squeezing/antisqueezing extraction below 0.5 dB has relatively poor accuracy, but this does not affect the overall qumode spectrum envelopes.
The relative frequencies of the qumodes, i.e., relative qumode spectrum, can be obtained by identifying the centers of the antisqueezing line shapes via Lorentzian fitting. The average root mean square deviation of the fitting is only 0.15 dB, showing an excellent agreement between fitting and measurements. \({{\Delta }}{\omega }_{N}^{Q}\) of all the qumodes are plotted in Fig. 4d, and their deviations from equidistant are within the 5 MHz spectroscopy resolution limit for the entire 1 THz optical span of the quantum microcomb. The qumode spectrum overlaps well with the twosided averaged cold cavity mode spectrum, −(Δω_{N} + Δω_{−N})/2, which represents the averaged deviation from equidistant of the cold cavity mode N and −N. It should be noted that in the qumode spectrum measurement, the cavity is pumped by >100 mW power, which could alter the cavity mode spectrum through thermooptic effect and self/crossphase modulation effects. Further study in the future is necessary to understand the requirement for perfectly equidistant frequencies of qumodes. In this measurement, the cavity escape efficiency is adjusted to 77% to achieve a more stable coupling condition as the entire measurement spans over 18 hours. As a result, the amount of squeezing/antisqueezing at δ = 0 MHz is different from that in the Fig. 2. In this experiment, the escape efficiency is adjusted by varying the relative position between the microresonator and the tapered fiber^{68}. The stability of the escape efficiency can be dramatically improved by packaging the microresonator systems^{69}, or by integrating the coupling waveguide and the resonator on the same chip^{67}.
Discussion
In summary, we have demonstrated a deterministic twomodesqueezed quantum microcomb in a silica microresonator on a silicon chip. The generation of squeezed microcomb is not limited to Kerr microresonators, but can also be realized in microresonatorbased χ^{(2)} parametric oscillators^{70,71,72,73}. For our system, the raw squeezing can be improved in the future by reducing system losses, improving photodiode quantum efficiency, and achieving higher resonatorwaveguide escape efficiency. The number of measurable qumodes, 40, is primarily limited by the span of the local oscillator, and this could be dramatically increased in the future by spectrum broadening of the EOM comb^{60}, or by using broadband dissipative Kerr soliton microcombs^{6} as the LOs. The optical span of quantum microcombs will ultimately be limited by the microresonator dispersion, which sets the bandwidth of Kerr parametric gain. Through dispersion engineering, Kerr parametric sidebands that are ~ ±80 THz away from the pump frequency have been reported in microresonators^{74}, which indicates the possibility of creating hundreds or thousands of qumodes in a single microresonator. The miniaturization of deterministic quantum frequency combs provides a path towards mass production, which could be critical for applications in quantum computing, quantum metrology, and quantum sensing^{75,76}.
Methods
Experimental setup
The experimental setup is shown in Fig. 5a. A continuouswave (cw) laser (New Focus, TLB6700) at 1550.5 nm is used to drive both the squeezed microcomb and the LOs. For the squeezed microcomb generation, the cw laser is amplified by an EDFA to pump the Kerr microresonator. A FBG filter is used to filter out the ASE noise from the EDFA. The amplified pump laser is then coupled into the microresonator through a singlemode tapered fiber. At the through port of the tapered fiber, another FBG filter is used to separate light at the pump laser wavelength from light at all other wavelengths. The transmitted squeezed microcomb from the FBG is sent to a 50/50 fiber coupler to be combined with the LOs for balanced homodyne detection. In the experiment, the PDH locking technique is used to lock the pump laser frequency to the resonator mode frequency by servo control of the cwlaser frequency. This is implemented by phase modulating the pump laser before the EDFA with an electrooptic PM, and then photodetecting the pump laser after the second FBG filter. The phase modulation frequency is set to 80 MHz, much higher than the resonator linewidth. It should be noted that the Brillouin scattering does not affect the squeezing process in our resonator, as the resonator FSR is designed to be completely out of the Brillouin gain bandwidth^{58}. Raman scattering in silica has its peak gain at 13 THz away from the pump, and the peak Raman gain is smaller than the Kerr parametric gain in microresonators with anomalous dispersion^{1}. As the optical span of the quantum microcomb is only ±0.5 THz around the pump, the Raman gain within our microcomb span is only ~2% of the peak Raman gain, and it has a negligible effect in our current experiment. The effect of Raman scattering on wideband quantum microcombs will be studied in the future.
Electrooptic modulation frequency comb
The LOs in this experiment are derived from an EOM frequency comb^{77}. The EOM comb is convenient to create coherent LOs which are hundreds of GHz apart from the pump laser frequency. In our EOM comb, the cw laser is amplified by an EDFA to 200 mW and is phase modulated by three cascaded electrooptic PMs at frequency f_{m}, which is provided by a signal generator (Keysight, PSG E8257D). The modulators are driven by amplified electrical signals that are synchronized by electrical phase shifters (PSs). The output power of the electrical amplifiers (Amps) is ~33 dBm. As the EOM comb and the microresonator share the same pump laser, the LOs derived from the EOM comb are inherently coherent with the squeezed microcomb. A typical EOM comb spectrum is shown in Fig. 5b (blue line), and the cw pump laser spectrum (black) is also shown as a reference. The EOM comb is then sent to a programmable linebyline waveshaper (Finisar 1000A, filter bandwidth setting resolution: ±5 GHz), which can control the amplitude and phase of each EOM comb line. To measure the noise variance of qumodes (−N, N), the waveshaper is set to only pass the comb lines whose frequencies are ±N × FSR apart from the pump laser. As an example, the LOs for qumodes (−21, 21) are shown in Fig. 5b (red line). Finally, the LOs are amplified to ~17 mW and are combined with the squeezed microcomb for balanced homodyne detection. It should be noted that the relative phase between the local oscillator and the squeezed field could be different from the phase shift applied by the PM in the LO optical path. This is because environmental fluctuations, e.g., ambient temperature, can cause phase variations in fibers in both LO and squeezed light paths. Finally, the electrical amplifiers in the EOM comb cutoff at 18 GHz, which is smaller than the FSR of the resonator (represented by f_{r}). As a result, the EOM modulation frequency, f_{m}, is set to n/m × f_{r}, such that the frequency of the mth EOM comb line can align with that of the nth resonator mode. The modulation frequencies used in the experiment are: f_{m} = 3/4 × f_{r} = 16.464438 GHz for mode pairs ±6, ±9, ±12, ±15, ±18, and ±21; f_{m} = 2/3 × f_{r} = 14.635056 GHz for mode pairs ±4, ±8, ±14, ±16, and ±20. For mode pairs of ±5, ±7, ±11, ±13, ±17, ±19, ±22, and ±23, modulation frequencies of: 5/7 × f_{r} = 15.680417 GHz, 7/9 × f_{r} = 17.074232 GHz, 11/15 × f_{r} = 16.098562 GHz, 13/17 × f_{r} = 16.787270 GHz, 17/23 × f_{r} = 16.225823 GHz, 19/25 × f_{r} = 16.683964 GHz, 22/29 × f_{r} = 16.653684 GHz, and 23/29 × f_{r} = 17.410670 GHz are used, respectively.
The phase noise of the signal generator that drives the EOM comb contributes to the phase fluctuation of the local oscillator, which could potentially affect squeezing measurement^{78}. Here, we estimate its impact on our experiments. The root mean square (RMS) of phase jitter from the signal generator can be calculated from its singlesideband phase noise by integrating the phase noise from the electrical spectrum analyzer (ESA) VBW used in the squeezing measurement (100 Hz), to the bandwidth of our balanced photodetection circuit (250 MHz). The RMS of phase jitter (\(\widetilde{\theta }\)) is calculated to be 0.0024 rad (0.14°) for comb mode 1 (~22 GHz), and is 0.055 rad (3.2°) for comb mode 23 (~0.5 THz). After taking account of this phase fluctuation, the observable level of squeezing^{78} is \(R^{\prime} \,\approx\, {R}_{{{{{\mbox{S}}}}}}{\cos }^{2}\widetilde{\theta }\,+\,{R}_{{{{{\mbox{AS}}}}}}{\sin }^{2}\widetilde{\theta }\), where R_{S} and R_{AS} are the variance of output squeezing and antisqueezing, respectively. For the current experimental condition, assuming 2 (7) dB squeezing (antisqueezing) at mode 4, and 1 (5) dB squeezing (antisqueezing) at mode 23 after optical losses, the phase fluctuation will cause the measured squeezing (\(R^{\prime}\)) to be 0.003 and 0.04 dB lower than the actual squeezing (R_{S}) at mode 4 and mode 23, respectively. It should be noted that the Nth comb line in the EOM comb has N times the RMS phase jitter of the 1st comb line in the EOM comb. Therefore, when scaling up the number of comb lines in an EOM comb through supercontinuum generation^{60} for squeezing measurement, the phase noise of the signal generator should be improved accordingly to maintain the low phase fluctuation of the LOs. A possible way to obtain exceptional phase noise performance for the EOM comb is through electrooptical frequency division, where the signal generator is synchronized to stable optical references^{79}.
Characterization of balanced photodiodes
In the twomode squeezing noise variance measurement, the balanced photodiodes (JDSU, ETX 300T) are operated in the shot noiselimited regime. The electrical circuit for balancing the photodiodes is homebuilt^{21}, and a commonmode rejection ratio of 31 dB is measured. The shot noiselimited regime is verified by the linear relationship between the noise power of the balanced photodiodes and the optical input power, which is shown in Fig. 6a. The measurement is done at 2.7 MHz with 100 kHz RBW. The electrical spectra from the balanced photodiodes at different optical input powers are shown in Fig. 6b. The resonance peaks in the dark noise are likely caused by the electrical circuits in the balanced photodiodes. At 16.6 mW input power, the electrical spectrum is relatively flat. The spectra rolloff is around 20 MHz.
Dependence of squeezing on optical pump power
The dependence of squeezing and antisqueezing on optical pump power is measured for qumode (−4, 4) and is presented in Fig. 6c. Ideally, when there is no optical loss, vacuum squeezing should increase with the pump power until the pump power reaches the OPO threshold. However, as the amount of squeezing in our experiment is primarily limited by optical losses, the increase of squeezing can no longer be observed when the pump power is roughly above half of the OPO threshold. On the other hand, the antisqueezing increases with the pump power. This observation is consistent with measurements in previous reports^{55}.
Data availability
Source data for Figs. 2–6 can be accessed at https://doi.org/10.6084/m9.figshare.14921670. Additional information is available from the corresponding author upon reasonable request.
Code availability
The codes that support the findings of this study are available from the corresponding authors upon reasonable request.
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Acknowledgements
The authors thank A. Beling at UVA for the access of signal generator, Y. Shen and J. Campbell at UVA for assisting photodiode quantum efficiency calibration, and gratefully acknowledge National Science Foundation.
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X.Y., O.P., Z.Y., and M.J. conceived the idea and designed the experiments. Z.Y. and M.J. performed the measurements. D.J. and H.L. fabricated the microresonator. X.Y., O.P., Z.Y. M.J., and S.S. analyzed the data. All authors participated in preparing the paper and contributed to the discussions. X.Y. supervised the project.
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Yang, Z., Jahanbozorgi, M., Jeong, D. et al. A squeezed quantum microcomb on a chip. Nat Commun 12, 4781 (2021). https://doi.org/10.1038/s4146702125054z
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DOI: https://doi.org/10.1038/s4146702125054z
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