Millimeter wave (mmWave) generation using photonic techniques has so far been limited to the use of near-infrared lasers that are down-converted to the mmWave region. However, such methodologies do not currently benefit from a monolithic architecture and suffer from the quantum defect i.e. the difference in photon energies between the near-infrared and mmWave region, which can ultimately limit the conversion efficiency. Miniaturized terahertz (THz) quantum cascade lasers (QCLs) have inherent advantages in this respect: their low energy photons, ultrafast gain relaxation and high nonlinearities open up the possibility of innovatively integrating both laser action and mmWave generation in a single device. Here, we demonstrate intracavity mmWave generation within THz QCLs over the unprecedented range of 25 GHz to 500 GHz. Through ultrafast time resolved techniques, we highlight the importance of modal phases and that the process is a result of a giant second-order nonlinearity combined with a phase matched process between the THz and mmWave emission. Importantly, this work opens up the possibility of compact, low noise mmWave generation using modelocked THz frequency combs.
The ability to generate millimetre (mmWave) waves (30–300 GHz) from highly stable lasers promises to be a key method to achieve the spectrally pure, low phase noise and microwave signals that are targeted for local oscillators in high frequency communications1,2,3. Examples have been shown by heterodyning two optical lasers4, opto-electronic oscillators5 and pulsed lasers6, in a nonlinear medium or a fast photodetector to generate microwaves signals. This field of microwave photonics has also been revolutionised by the advent of the optical frequency comb, where the beating of the highly stable modes can generate low noise and high purity microwave emission7,8,9. Most of these methods, however, use lasers operating in the visible or near-infra-red part of the electromagnetic spectrum, leading to orders of magnitude difference in photon energy between the generating laser photon energy and that of the microwave photon – the quantum defect. This inherently limits the efficiency of the system ~ EGHz/Eopt, where Eopt is typically 1 eV and EGHz < 1 meV. Finally, microwave photonic systems based on optical frequency combs are typically used in a non-integrated approach, where the optical laser is separated from the fast photo-mixer or nonlinear crystal7,9,10. Although a range of electronic methods can be used to generate directly or through upconversion mmWave emission11,12,13, these sources typically suffer from high phase noise and therefore not as spectrally pure as photonic based sources7,14. In this work we show that Terahertz (THz) frequency quantum cascade lasers (QCLs)15, with their inherently low photon energies, two orders of magnitude smaller than in the optical range, can be used as an integrated platform to generate free space emission over the entire mmWave region (0.02–500 GHz) via intracavity nonlinear beating of the laser longitudinal modes.
THz QCLs operate between 1.2 and 5 THz, corresponding to photon energies of 5–21 meV, and possess ultrafast dynamics and giant nonlinearities16 permitting an integrated approach where the laser excitation and mmWave generation are realised within the same laser cavity. THz QCLs have achieved impressive performances in term of spectral coverage17, output power18 and bandwidth19,20 via carefully designed waveguides and active regions. Further, temperature operation has been extended to Peltier cooled operation21,22, with recent results showing operation up to 250 K23 with further perspectives to achieve room temperature operation through new bandstructure designs and materials24. To extend the capabilities of these devices, nonlinear intracavity processes have been successfully exploited to generate frequencies in the telecom band ~1.55 µm25,26, and shown the generation of frequency combs27,28,29 with octave spanning bandwidth20. Furthermore, difference-frequency generation (DFG) in mid-infrared QCLs has shown the possibility of efficient THz generation at room temperature30,31,32,33. These demonstrations illustrate the giant optical nonlinearities that can occur within QCLs (greater than ~105 pm/V, compared to 102 pm/V for GaAs) and how they can be used to access different spectral regions. However, the possibility of accessing the entire mmWave region, either through direct or nonlinear generation, has yet to be demonstrated. Recently, mid-infrared QCL-based frequency combs were shown to generate free space microwave radiation through beating of the comb lines in an integrated approach34,35. This takes advantage of the fast QCL dynamics (~1 ps), suggesting potential operation even up to THz frequencies, and highlighted both electronic and photonic methods to generate electromagnetic radiation within QCLs. However, such microwave emission has, so far, been limited to low frequencies with optical beatnote detection up to 13 GHz shown on a Schottky mixer36. This results in a large spectral gap between 15 and 500 GHz for QCL-based microwave generation.
Here we demonstrate free space mmWave generation in a set of THz QCLs with different dimensions, emission bandwidth and spectral response. As a common characteristic, all devices show mmWave emission lines, equally spaced in frequency by the QCL round-trip frequency. Depending on the bandwidth of the THz QCL employed and the dispersion of the THz lines, we realise mmWave emission up to 500 GHz. Moreover, we demonstrate that the frequency of the mmWave lines can be engineered by designing a QCL with two-separated THz spectral bands, with the formation of the mmWave emission measured on ultrafast timescales. We also highlight the important role of modal phases for DFG and we show here that the mmWave generation is a result of a phase matched process, owing to low loss waveguides and to the phase of the mmWave emission being equal to the envelope of the THz emission. Finally, we show a giant second-order nonlinearity from the QCL bandstructure, owing to the closely spaced sublevels in energy that directly permits a nonlinearity in the mmWave range. This could support the stabilisation of QCL-based frequency combs, in addition to four-wave mixing.
To characterise the entire QCL emission from 10 to 4000 GHz, we employ an injection seeding technique based around electro-optic detection in a THz-TDS system. As well as enabling ultrafast time-resolved measurements, this proven technique provides a detection bandwidth much greater than spectrum analysers and limited only by the cut-off frequency of the ZnTe electro-optic detection crystal37. To demonstrate mmWave generation, a coherent terahertz pulse generated from an ultrafast laser is injected into the QCL, and at the same time it is switched on with an ultrafast electrical pulse that is synchronised to the THz pulse. The pulse is amplified to the steady state where it seeds the QCL emission. This permits free space coherent detection of the QCL time-resolved electric field using a second beam from the same ultrafast laser38. The technique has shown to be equivalent to laser action on the inherent QCL spontaneous emission such that the measured time profile corresponds to the free-running case39. A squared Fourier transform operation is applied to the measured time-domain trace in order to extract the QCL intensity spectrum. In this study, three QCLs with lasing frequencies between 2 and 3 THz with metal-metal waveguides40,41 were used. For QCL1 and QCL3, the active region design is based on a 2.4-THz three well42,43 structure, whilst QCL2 is based on a 2.8-THz heterogeneous stacked nine well design29,44,45 for broadband operation (~800 GHz). QCL1 shows laser action with a bandwidth of ~500 GHz and is 1.5 mm long and 60 µm wide. QCL2 is 2.9 mm long and 85 µm wide. Finally, QCL3 was designed for two lasing bands separated by ~240 GHz using an integrated Gires-Tournois interferometer46 (GTI) and is 3 mm long and 68 µm wide. The GTI is 60 µm long, and separated from the main QCL section by 4 µm. Each QCL is used to show a range of spectral responses in the mmWave generation as discussed below.
The emission properties of QCL1 are shown in Fig. 1. The temporal response (Fig. 1a) shows the typical profile from these devices38,43 with a strong amplitude modulation that can arise from the QCL ultrafast dynamics39. The corresponding frequency spectrum (Fig. 1b) shows emission centred at 2.42 THz with Fabry-Pérot modes separated by the round-trip frequency (fRT). Owing to the broadband nature of the coherent detection, the spectrum also clearly shows spectral modes covering the mmWave region between 26 GHz and 367 GHz, also separated by exactly fRT. In order to rule out any spectral artefact originating from nonlinearities in the measurement arrangement that are not associated with the QCL, we additionally conducted the investigations employing a 500-GHz low-pass filter (Spectrasil B). The transmission spectrum is shown in Fig. 1b (blue dotted curve). Although the THz signal intensity is attenuated by more than one order of magnitude, the mmWave lines remain the same, demonstrating that the emission originates from the QCL. An expanded view of the mmWave spectrum is shown in Fig. 2. Two observations can be made. First, there is an equal mode spacing between the THz and the mmWave lines (~ 26 GHz), with the latter’s bandwidth limited to the bandwidth of the THz emission. Second, the position and intensity of the mmWave lines can be evaluated by calculating the expected positions from the measured THz temporal emission whilst assuming a second-order nonlinearity for DFG. This is done by calculating the Fourier transform of the square of the THz temporal emission (blue curve in Fig. 2), as the second-order polarisation, P2nd, is proportional to the square of the electric field, E(t). This allows the phase of each mode to be automatically considered in the calculated emission spectrum. The effect of the phase is discussed further below in the case of QCL2. The collection and detection efficiencies are included in the calculation and were estimated by 3D simulations of the far-field (COMSOL Multiphysics) and the waist size of each frequency at the detection crystal, respectively. These factors lead to reduced detection response to low-frequency mmWave emission and further details are highlighted in the supplementary material Figs. 2 and 3. Figure 2 shows an excellent coincidence with the frequencies of the mmWave and reasonable agreement with intensities of the mmWave modes with the lowest modes showing weak emission. Indeed, the fundamental mode at ~ 26 GHz is barely observed, although the second harmonic is weaker than the third, in contrast to the simulations. The detection of the fundamental electrical beatnote is discussed further below.
As well as simulating the expected spectrum, a power dependence measurement was performed to further show that the mechanism is based on a second-order nonlinearity. From the spectrum acquired from the temporal trace, the integral of the mmWave spectrum as a function of the integrated THz intensity was measured, with the THz intensity varied with the QCL bias (see Fig. 3). A power law is used to fit the experimental data and the best agreement is found for a value of the exponent 2.10 ± 0.33. This identifies the second-order nonlinear susceptibility, χ(2), as the main contribution to the nonlinear optical process. The small deviation from an exponent equal to 2 is most likely a result of not efficiently detecting the low harmonics. To conclude, QCL1 shows equally spaced mmWave lines from 25 to 367 GHz with an agreement between the mode intensity distribution of the measured and the calculated GHz lines through a second-order nonlinearity.
With the proof of principle of mmWave DFG demonstrated, QCL2, designed for ultra broadband THz emission, showed mmWave generation with an increased bandwidth extending to 500 GHz (see Fig. 4a). However, owing to the irregular power distribution between the THz QCL Fabry-Pérot modes, the mmWave modal distribution is also irregular, in agreement with the simulations shown in Fig. 4b (blue curve), calculated as described above. Here, the expected spectrum is further compared to the case where the phases of the modes are assumed to be equal (black curve). Although the frequencies are the same, the modal intensities at low frequencies (<100 GHz) are considerably higher than those measured. This highlights strongly the effect of the modal phases on the difference-frequency generation process in the case of neighbouring Fabry-Pérot modes. Furthermore, similar to observations in QCL1, QCL2 demonstrated that the mmWave modes at low frequencies were weak compared to that expected, with the fundamental mode missing. However, as QCL2 was 3 mm long, the electrical and free-space fundamental beatnote is expected to be around 13 GHz. This was then electrically detected36, using the QCL itself as an ultrafast detector and a standard spectral analyser (inset Fig. 4a), despite it being missing in the free space spectrum. This supports the above simulations for QCL1 that the free space optical modes at lower frequencies are not efficiently detected. This is a result of the strong diffraction owing to the subwavelength dimensions of the QCL waveguide, large focused spot sizes at these frequencies, combined with THz optics (parabolic mirrors) that have a limited collection efficiency. The detection of the narrow electrical beatnote also suggests a coherence between the Fabry-Pérot modes, which can be potentially locked to an external reference for modelocking. The high frequency microwave signals would also possess similar coherence properties.
For the final sample, QCL3, we show how the mmWave emission can be controlled to emit predominately at a single frequency by engineering the THz QCL spectral emission using dispersion management. Research using MIR QCLs30 has exploited imbedded gratings to force the QCL to emit at two distinct spectral lines for THz generation by DFG. Here we designed a THz QCL with an integrated GTI46 that permits the QCL to lase on distinct and separated spectral bands. Where previous work was based on placing the GTI off-resonance to reduce the total dispersion, here the centre of the QCL emission is placed in a dispersive regime that permits the generation of the spectral bands. The same active region as in QCL1 was used with a GTI of length 60 µm. The full emission spectrum of QCL3 is shown in Fig. 5a showing both the mmWave DFG and the THz emission. Figure 5b shows an expanded view of the THz spectra, where the THz QCL emits in two THz spectral bands, each spanning several tens of gigahertz. The highest intensity modes are at 2.586 THz and 2.342 THz with a frequency separation of 0.244 THz. An expanded view of the mmWave spectra is shown in Fig. 5c where the spectral position of the mmWave signal is in exact agreement with the difference in the frequencies of the main THz peaks. The intensity of the mmWave emission is equal to 0.02 percent of the highest pump intensity at 2.586 THz. This demonstrates the possibility of tailoring the desired mmWave spectrum by carefully engineering the THz emission, opening up the possibility of extending the emission towards 1 THz using octave spanning QCLs. With QCL3 showing strong emission at mmWave frequencies, the time evolution of the spectrum was studied and shown in Fig. 6 as a colour plot. The intensities of the modes are plotted as a function of frequency (x) and time in femtoseconds (y-axis). This shows clearly that the mmWave emission (left curve) only takes hold after the QCL emission (right curve) is established and stable, here from ~400 ps. Figure 6 also shows the interesting dynamics of the system where before 400 ps corresponds to the initial transient stage where all modes experience some gain and hence amplified over a few round trips. Here it can be seen that the modes in-between the two main parts of the spectrum experience less gain owing to the GTI reflectivity. After 400 ps the laser reaches a steady-state region corresponding to laser action and where the cavity (GTI+laser) establishes the spectral emission. This behaviour is similar to the dynamics observed in DFB THz QCLs47, which was compared to a reduced rate formulism.
Finally, the efficiency of the process can be used to determine the origin and the nonlinear susceptibility arising from difference-frequency generation25,30. The efficiency of QCL1, defined here as the ratio between the integrated mmWave and the THz spectrum, was found to be ~1.7 × 10−4. Previously work has indicated the possibility of phase matching in measurements of the microwave transmission48 and pulse generation in THz QCLs43,49. Here, using the time resolved nature of our experimental technique, we show directly the process is phase matched between the THz QCL emission and the nonlinear mmWave generation. Figure 7a shows the electric field of the THz QCL emission and the mmWave emission in the seeded regime. It is clear that the mmWave emission is in phase with the envelope of the THz emission, i.e., the phase velocity of the former is equal to the group velocity of the latter. This is a result of the low dispersion between these spectral ranges compared to the mid- and near-infra-red and the relatively low mmWave losses in these microstrip-type waveguides. Taking this phase matched process, from the efficiency a second-order susceptibility χ(2) ~ 1 × 105 pm/V over the mmWave region is estimated with a THz intracavity power of ~20 mW. This giant nonlinearity when compared to GaAs (~100 pm/V) is comparable to other intersubband systems and is a result of the large dipoles between closely spaced subbands32. Indeed the calculated value from the QCL bandstructure30 is χ(2) ~ 6 × 105 pm/V, highlighting that the nonlinearity is a result of resonant excitations of the subbands (see Fig. 7b and supplementary material Fig. 4 for details on the simulation). The measured susceptibility is lower and could be a result of the lack of sensitivity of the detection scheme to low microwave frequencies as discussed above. Further, all the carrier population is assumed to be in the upper laser that tends to overestimate the nonlinearity. By engineering the dipole and nonlinear interferences between subbands50, further perspectives to engineer the response of the mmWave emission for higher efficiencies are possible.
To conclude, we demonstrate the generation of narrowband free space mmWave radiation that can cover the entire 26–500 GHz range. This is based on the beating of the Fabry-Pérot modes of THz QCLs and using electro-optic detection for sensitivity over the full microwave, mmWave and THz regions. A range of functionalities were shown with regular mode spacing up to 367 GHz, mmWaves generated up to 500 GHz using broadband QCLs and engineering of the mmWave emission by using integrated GTIs. The generation process was shown to rely on a second order process and thus indicates a second-order nonlinearity. The down-conversion of THz frequency lines into microwave and sub-THz emission is also a promising process to achieve continuous emission from a few GHz to several THz using multi-octave spanning QCLs. Further, owing to the demonstrated frequency comb nature of these sources and the increasing temperature operation of THz QCLs, the generation of extremely low-noise mmWave emission at hundreds of GHz is feasible. This would potentially permit the application of these sources as local oscillators for future high-frequency free space telecommunications.
The temporal characterisation of the THz quantum cascade laser (QCL) is based on coherent sampling of the electric field (E-field) using electro-optic detection. This technique requires the emission of the THz QCL to be phase locked to a THz pulse, and thus locked to the repetition rate of a femtosecond laser. An established ultrafast injection seeding technique is employed to realise this condition. A broadband THz seed pulse with a fixed phase is generated using an interdigitated photoconductive switch excited by a femtosecond Ti:Sapphire laser (see supplementary fig. 1)51. The THz pulse is injected into one end of the QCL cavity as an electrical radio frequency (RF) pulse (duration of a few nanoseconds), synchronised with the seed pulse, is used to gain switch the QCL. This permits the THz input pulse to be amplified, eventually seeding the QCL emission, avoiding laser action on the QCL’s inherent spontaneous emission. The QCL emission is then measured using electro-optic sampling using a ZnTe crystal and a second beam from the same Ti:Sapphire laser.
The datasets generated and analysed during the current study are available in the zenodo repository, https://doi.org/10.5281/zenodo.4384637
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The authors acknowledge funding from European Union under the Horizon 2020 research and innovation programmes FET-Open grant ULTRAQCL 665158, the European Research Council (ERC) consolidator grants SPRINT (681379) and LEON (820133), the French National Research Agency (ANR-18-CE24-0013-02 - “TERASEL”), and EPSRC programme ‘HyperTerahertz’ (EP/P021859/1). E.H.L. acknowledges support from the Royal Society and the Wolfson Foundation.
The authors declare no competing interests.
Peer review information Nature Communications thanks Manfred Helm and the other anonymous reviewers for their contribution to the peer review of this work.
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Pistore, V., Nong, H., Vigneron, PB. et al. Millimeter wave photonics with terahertz semiconductor lasers. Nat Commun 12, 1427 (2021). https://doi.org/10.1038/s41467-021-21659-6