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Frequency combs induced by optical feedback and harmonic order tunability in quantum cascade lasers: supplementary materials

Carlo Silvestri School of Electrical Engineering and Computer Science, The University of Queensland, Brisbane, QLD 4072, Australia    Xiaoqiong Qi School of Electrical Engineering and Computer Science, The University of Queensland, Brisbane, QLD 4072, Australia    Thomas Taimre School of Mathematics and Physics, The University of Queensland, Brisbane, QLD 4072, Australia    Aleksandar D. Rakić School of Electrical Engineering and Computer Science, The University of Queensland, Brisbane, QLD 4072, Australia
preprint: AIP/123-QED

S.1 Effective semiconductor Maxwell-Bloch equations with optical feedback

We study the quantum cascade laser (QCL) dynamics by using a full set of effective semiconductor Maxwell–Bloch equations (ESMBEs) for the Fabry–Perot (FP) configuration.Silvestri20; Silvestri22; SilvestriCLEO This model is based on a phenomenological expression for the optical susceptibility of a QCL active medium, and it encompasses the main properties of semiconductor materials such as a non null α\alpha factor, a dependence of the susceptibility from the density of carriers, asymmetric gain and refractive index spectra, and nonlinearities at each order, such as Kerr effect and four-wave mixing. In the case of FP cavity it also accounts for SHB through the inclusion of a carrier grating. The ESMBEs read:

E+z+1vE+t\displaystyle\frac{\partial E^{+}}{\partial z}+\frac{1}{v}\frac{\partial E^{+}}{\partial t} =\displaystyle= αL2E++gP0+,\displaystyle-\frac{\alpha_{\mathrm{L}}}{2}E^{+}+gP_{0}^{+}, (S.1)
Ez+1vEt\displaystyle-\frac{\partial E^{-}}{\partial z}+\frac{1}{v}\frac{\partial E^{-}}{\partial t} =\displaystyle= αL2E+gP0,\displaystyle-\frac{\alpha_{\mathrm{L}}}{2}E^{-}+gP_{0}^{-}, (S.2)
P0+t\displaystyle\frac{\partial P_{0}^{+}}{\partial t} =\displaystyle= πδhom(1+iα)[P0++if0ε0εb(1+iα)(N0E++N1+E)],\displaystyle\mathrm{\pi\delta_{hom}}(1+i\alpha)\left[-P_{0}^{+}+if_{0}\varepsilon_{0}\varepsilon_{\mathrm{b}}\left(1+i\alpha\right)\left(N_{0}E^{+}+N_{1}^{+}E^{-}\right)\right], (S.3)
P0t\displaystyle\frac{\partial P_{0}^{-}}{\partial t} =\displaystyle= πδhom(1+iα)[P0+if0ε0εb(1+iα)(N0E+N1E+)],\displaystyle\mathrm{\pi\delta_{hom}}(1+i\alpha)\left[-P_{0}^{-}+if_{0}\varepsilon_{0}\varepsilon_{\mathrm{b}}\left(1+i\alpha\right)\left(N_{0}E^{-}+N_{1}^{-}E^{+}\right)\right], (S.4)
N0t\displaystyle\frac{\partial N_{0}}{\partial t} =\displaystyle= IeVN0τe+i4[E+P0++EP0E+P0+EP0],\displaystyle\frac{I}{eV}-\frac{N_{0}}{\tau_{\mathrm{e}}}+\frac{i}{4\hbar}\left[E^{+*}P_{0}^{+}+E^{-*}P_{0}^{-}-E^{+}P_{0}^{+*}-E^{-}P_{0}^{-*}\right], (S.5)
N1+t\displaystyle\frac{\partial N_{1}^{+}}{\partial t} =\displaystyle= N1+τe+i4[EP0+E+P0].\displaystyle-\frac{N_{1}^{+}}{\tau_{\mathrm{e}}}+\frac{i}{4\hbar}\left[E^{-*}P_{0}^{+}-E^{+}P_{0}^{-*}\right]. (S.6)

where E+(z,t)E^{+}(z,t), E(z,t)E^{-}(z,t) are the forward and backward electric fields, P0+P_{0}^{+}, P0P_{0}^{-} are the forward and backward polarization terms, N0N_{0} is the zero-order density of carriers, and N1+N_{1}^{+}, N1N_{1}^{-} are the first-order terms of the density of carriers, reproducing the carrier grating due to SHB; vv is the group velocity, αL\alpha_{\mathrm{L}} is the loss coefficient, α\alpha is the linewidth enhancement factor, δhom\delta_{\mathrm{{hom}}} is the homogeneous part of the gain bandwidth, f0f_{0} is the differential gain, ε0\varepsilon_{0} is the dielectric permittivity of the vacuum, εb\varepsilon_{\mathrm{b}} is the relative dielectric constant of the QCL active medium, II is the driving current of the laser, VV is the volume of the active region, τe\tau_{\mathrm{e}} is the carrier lifetime, and the coefficient gg is given by:

g=iω0NpΓc2ε0nrc,g=\frac{-i\omega_{0}N_{\mathrm{p}}\Gamma_{\mathrm{c}}}{2\varepsilon_{0}n_{\mathrm{r}}c}\,, (S.7)

where NpN_{\mathrm{p}} is the number of stages of structure, ω0\omega_{0} is the cold cavity angular frequency closest to the gain peak and it is used as a reference frequency, Γc\Gamma_{\mathrm{c}} is the optical confinement factor, cc is the speed of light in the vacuum, and nrn_{\mathrm{r}} is the effective background refractive index of the medium. We remark that δhom\delta_{\mathrm{hom}} is related to the polarization dephasing time τd\tau_{\mathrm{d}} through the equation δhom=1πτd\delta_{\mathrm{hom}}=\frac{1}{\pi\tau_{\mathrm{d}}}.Silvestri20
We want to include the effect of the optical feedback in the boundary conditions of the model. Therefore, we start by adding a term Efb(t)E_{\mathrm{fb}}(t) to the free-running boundary conditions, corresponding to an external target placed at distance LextL_{\mathrm{ext}} from right facet of the QCL:

E(L,t)\displaystyle E^{-}(L,t) =\displaystyle= RE+(L,t)+Efb(t),\displaystyle\sqrt{R}E^{+}(L,t)+E_{\mathrm{fb}}(t), (S.8)
E+(0,t)\displaystyle E^{+}(0,t) =\displaystyle= RE(0,t),\displaystyle\sqrt{R}E^{-}(0,t), (S.9)

where LL is the QCL cavity length and RR is the reflectivity of each facet of the QCL. We want to determine Efb(t)E_{\mathrm{fb}}(t). In the frequency domain we can write the reflection coefficient due to the external feedback in our configuration as:

r(ω)=rexttL2eiΦextei(ωω0)τext\displaystyle r(\omega)=r_{\mathrm{ext}}t_{\mathrm{L}}^{2}e^{-i\Phi_{\mathrm{ext}}}e^{-i(\omega-\omega_{0})\tau_{\mathrm{ext}}} (S.10)

where ω\omega is the angular frequency, tLt_{\mathrm{L}} is the field transmissivity for both outgoing and incoming field, Φext=2Lextω0/c\Phi_{\mathrm{ext}}=2L_{\mathrm{ext}}\omega_{0}/c, τext=2Lext/c\tau_{\mathrm{ext}}=2L_{\mathrm{ext}}/c, rextr_{\mathrm{ext}} is the frequency-independent reflectivity of the external target. If we calculate the Fourier transform of the forward field E+(L,t)E^{+}(L,t), we multiply it by r(ω)r(\omega) given by Eq. (S.10), and then we anti-transform the obtained product, we retrieve the following expression for the feedback term.Rimoldi22

Efb(t)=rexttL2E+(L,tτext)\displaystyle E_{\mathrm{fb}}(t)=r_{\mathrm{ext}}t_{\mathrm{L}}^{2}E^{+}\left(L,t-\tau_{\mathrm{ext}}\right) (S.11)

Since Eqs. (S.1)–(S.6) have been derived by assuming the frequencies of the multimode fields are referenced with respect to the central frequency ω0\omega_{0} (see ref.Silvestri20), we write Eq. (S.12) consistently with this hypothesis:

Efb(t)=rexttL2E+(L,tτext)eiω0τext\displaystyle E_{\mathrm{fb}}(t)=r_{\mathrm{ext}}t_{\mathrm{L}}^{2}E^{+}\left(L,t-\tau_{\mathrm{ext}}\right)e^{-i\omega_{0}\tau_{\mathrm{ext}}} (S.12)

If we also take into account the losses in the external cavity ϵL\epsilon_{\mathrm{L}}, and the ones due to the reinjection ϵS\epsilon_{\mathrm{S}}, we obtain the boundary conditions Eqs. (1)–(2) presented in the main manuscript.

S.2 Numerical study: procedure and methods

Length of the laser cavity L=2L=2 mm
Effective refractive index n=3.6n=3.6
Confinement factor Γc=0.13\Gamma_{c}=0.13
Mirror reflectivity R=0.3R=0.3
Differential gain f0=7×105μm3f_{0}=7\times 10^{-5}\mu\mathrm{m}^{3}
Volume of the active region V=3.6×106μm3V=3.6\times 10^{6}\mu\mathrm{m}^{3}
Number of stages Np=90N_{p}=90
Homogeneous gain bandwidth δhom=0.32\delta_{\mathrm{hom}}=0.32 THz
Waveguide loss αL=3.8cm1\alpha_{\mathrm{L}}=3.8~{}\mathrm{cm^{-1}}
Central emission frequency ν0=3\nu_{0}=3 THz
Linewidth enhancement factor varies
Carrier lifetime varies
Table 1: ESMBEs parameters. PiccardoReview; SilvestriReview; alphaneg; Silvestri22; Faist_2016; Li22; Li15; Vitiello2021

The values of the ESMBEs parameters exploited in this article are presented in Table I, and they are typical values for a THz QCL.SilvestriReview; PiccardoReview They have been used to study the free-running case in ref. Silvestri22, where two comb regions characterized by fundamental and second order harmonic combs were found.

Refer to caption
Figure S.1: Example of a performed simulation. For the first 4040~{}ns, the QCL is configured in free-running operation: after a time interval of about 3333 ns in which no power is emitted (i), the QCL starts to lase and reaches a stable single mode emission (ii); then, at t=40t=40 ns, the optical feedback is switched on, and the QCL transits on a different dynamical regime (iii).

The numerical study which leads to Fig. 2 presented in the main manuscript, is conducted according to the following points. The laser is initially configured in free running operation, i.e. we solve the ESMBEs by adopting the boundary conditions with ϵ=0\epsilon=0, and the value of the bias current is chosen in order to have single mode emission; in particular, we set I=1.08IthrI=1.08I_{\mathrm{thr}}. Once the QCL output reaches a stable single mode emission, at t=40t=40 ns the external target is introduced (Fig. S.1) by integrating the ESMBEs with the boundary conditions Eqs. (1)–(2), for fixed values of LextL_{\mathrm{ext}} and ϵ\epsilon. Each simulation has total duration of 1μs1\mu s and is performed for a pair (ϵ\epsilon, LextL_{\mathrm{ext}}); the set of values of ϵ\epsilon are chosen between 0.01 and 0.09 with step 0.01, and between 0.1 and 1 with step 0.1; the values of LextL_{\mathrm{ext}} are selected in four regions with a different step for each region: region 1 corresponds to the short cavity regime, and includes the values between 1 mm and 9 mm, with step 1 mm; region 2 includes the values between 1 cm and 9 cm, with step 1 cm; region 3 corresponds to LextL_{\mathrm{ext}} between 10 cm and 90 cm with step 10 cm; in region 4 we consider the long cavity regime, with the values 1 m, 2 m, and 3 m. This choice allows us to study the laser dynamics in different ranges of LextL_{\mathrm{ext}} with a limited number of simulations, providing a general overview of the laser behaviour under optical feedback.
The set of ESMBEs (S.1)-(S.6) with the boundary conditions (S.8)-(S.9) have been integrated using an optimized finite difference algorithm discretizing in both time and space, described in detail in the Appendix of Ref. Bardella17. The time step used in the simulations is dt=20dt=20~{}fs, which corresponds to a space step dz=1.8μdz=1.8~{}\mum. This leads to a duration for a single typical 1μ1~{}\mus long simulation of 5 hours on our Intel©\copyright Xeon©\copyright W-2145 CPU 3.70 GHz processor, with 64 GB RAM. However, we specify that the duration of the transients preceding the attainment of the steady state condition varies depending on the feedback parameters. This implies that simulations have slightly different durations from each other, and the values of 1 μ\mus and 5 hours are therefore indicative (average) values.

We would like to highlight that the study described in Section IV of the main manuscript follows the same procedure, with one difference: the bias current value is set to I=1.5IthrI=1.5I_{\mathrm{thr}}, which corresponds to a self-starting optical frequency comb regime. Therefore, we first simulate the free-running laser (ϵ=0\epsilon=0), allowing it to reach a steady state comb emission. Subsequently, we switch on the feedback and reproduce the map depicted in Fig. 5(a).

Finally, after solving the ESMBEs for each pair (ϵ\epsilon, LextL_{\mathrm{ext}}), we classify the obtained dynamical regimes following a rigorous procedure described in the following subsection.

S.2.1 Classification of the dynamical regimes

In order to classify the dynamical regimes, we filter the optical spectrum and we consider the modes within a 20dB power ratio to the spectral maximum. Let us name N20N_{20} the number of modes included in the -20dB bandwidth from the peak in the optical spectrum. If N20=1N_{20}=1, i.e. only the spectral maximum is included in 20dB-20~{}\mathrm{dB} spectral bandwidth, we classify the regime as a single mode emission.
If N20>1N_{20}>1, we compute the the comb indicators MσPM_{\sigma_{P}} and MΔΦM_{\Delta\Phi}, previously introduced and exploited in refs. Silvestri20; Silvestri22, which quantify respectively the power and phase noise, and allow us to understand if a regime is locked. Low values of these indicators correspond to low values of amplitude and phase noise, and therefore correspond to a frequency comb regime. We calculate them by filtering each line qq of the output optical field in the 20dB-20~{}\mathrm{dB} spectral bandwidth, and we retrieve the dynamics of the power of each line (Pq(t),q=1,,N20P_{q}(t),q=1,...,N_{20}) and the intermodal phase difference (ΔΦq(t),q=1,,N20\Delta\Phi_{q}(t),q=1,...,N_{20}). Then, we define the comb indicators by using the following equations:

MσP\displaystyle M_{\sigma_{P}} =\displaystyle= 1N20q=1N10σPq\displaystyle\frac{1}{N_{20}}\sum_{q=1}^{N_{10}}{\sigma_{P_{q}}} (S.13)
MΔΦ\displaystyle M_{\Delta\Phi} =\displaystyle= 1N20q=1N20σΔΦq,\displaystyle\frac{1}{N_{20}}\sum_{q=1}^{N_{20}}{\sigma_{\Delta\Phi_{q}}}, (S.14)

where:

μPq\displaystyle\mu_{P_{q}} =\displaystyle= Pq(t)\displaystyle\left\langle P_{q}(t)\right\rangle (S.15)
μΔΦq\displaystyle\mu_{\Delta\Phi_{q}} =\displaystyle= ΔΦq(t),\displaystyle\left\langle\Delta\Phi_{q}(t)\right\rangle, (S.16)
σPq\displaystyle\sigma_{P_{q}} =\displaystyle= (Pq(t)μPq)2\displaystyle\sqrt{\left\langle\left(P_{q}(t)-\mu_{P_{q}}\right)^{2}\right\rangle} (S.17)
σΔΦq\displaystyle\sigma_{\Delta\Phi_{q}} =\displaystyle= (ΔΦq(t)μΔΦq)2.\displaystyle\sqrt{\left\langle\left(\Delta\Phi_{q}(t)-\mu_{\Delta\Phi_{q}}\right)^{2}\right\rangle}. (S.18)

where the symbol \left\langle\right\rangle indicates the time average.
A this point, we use the following criterion to classify the simulated multimode states:

  • We define a simulated regime as an OFC if MσP<2102mWM_{\sigma_{P}}<2\cdot 10^{-2}\mathrm{mW} and MΔΦ<2102radM_{\Delta\Phi}<2\cdot 10^{-2}\mathrm{rad}, analogously to ref. Silvestri22.

  • If the simulated dynamics does not correspond to an OFC, we examine its optical spectrum. If the optical spectrum consists of a set of frequency bands whose central frequencies are the modes of the laser cavity, and whose spacing is the free spectral range of the external cavity FSRext\mathrm{FSR_{ext}}, we classify the regime as a mixed state.

  • If the simulated dynamics does not correspond to an OFC, and also does not satisfy the condition to be a mixed state, we classify it as an irregular regime.

S.3 Fine tuning of the external cavity length for a feedback-induced optical frequency comb (single mode as initial condition)

In this subsection we show that an OFC generated in regime of short cavity starting from a free-running CW, is sensitive to the phase accumulated in the external cavity. We shift external cavity by a quantity ΔLext\Delta L_{\mathrm{ext}} in the same order of the QCL central wavelength λ=100μ\lambda=100~{}\mum. In particular we consider integer multiples of λ/4\lambda/4. As example, in Fig. S.2 we show how the fundamental comb of Fig. 3(d) in the main manuscript evolves if we introduce a shift ΔLext=nλ/4\Delta L_{\mathrm{ext}}=n\lambda/4, with n=1,2,3,4=1,2,3,4, reporting alternance CW-OFC with period given by λ/2\lambda/2. We understand, therefore, that a π\pi phase accumulated in the external cavity (corresponding to λ/4\lambda/4 and 3λ/43\lambda/4) leads to a single-mode emission, while a 2π2\pi phase shift does not affect the comb emission. Therefore, the system is phase-sensitive, and this can be exploited for applications such as the detection of microscopic vibrations, or displacements.

Refer to caption
Figure S.2: Fine tuning of the EC cavity length LextL_{\mathrm{ext}} for the OFC of Fig. 3(d) in the main manuscript. Temporal evolution of the power for different values of Lext=Lext,0+nλ/4L_{\mathrm{ext}}=L_{\mathrm{ext,0}}+n\lambda/4, with n=1,2,3,4=1,2,3,4. Lext,0=7L_{\mathrm{ext,0}}=7~{}mm, ϵ2=36%\epsilon^{2}=36~{}\%, I=1.08IthrI=1.08I_{\mathrm{thr}}, other parameters as in Table 1.

Furthermore, we want to investigate how the comb emission is affected by a fine tuning of the external cavity length in the long cavity regime. If we keep ϵ2=36%\epsilon^{2}=36~{}\% as in the case of Fig. S.2, but we consider Lext,0=70L_{\mathrm{ext,0}}=70~{}cm, we report a mixed state emission. If also in this case we introduce a shift ΔLext=nλ/4\Delta L_{\mathrm{ext}}=n\lambda/4, with n=1,2,3,4=1,2,3,4 of the external cavity length, we report a mixed state for all the considered values of ΔLext\Delta L_{\mathrm{ext}}, as shown in Fig. S.3.

Refer to caption
Figure S.3: Fine tuning of the EC cavity length LextL_{\mathrm{ext}} in the long cavity regime for a mixed state case. Temporal evolution of the power for different values of Lext=Lext,0+nλ/4L_{\mathrm{ext}}=L_{\mathrm{ext,0}}+n\lambda/4, with n=1,2,3,4=1,2,3,4. Lext,0=70L_{\mathrm{ext,0}}=70~{}cm, ϵ2=36%\epsilon^{2}=36~{}\%, I=1.08IthrI=1.08I_{\mathrm{thr}}, other parameters as in Table 1.

At this point we want to examine how a feedback-induced comb is affected by a fine tuning of the external cavity length in the long cavity regime. For this reason, we consider Lext,0=30L_{\mathrm{ext,0}}=30~{}cm and ϵ2=1%\epsilon^{2}=1~{}\%, which corresponds to a frequency comb emission in the map of Fig. 2(a) in the main manuscript. By repeating the study performed for the two previous cases, we find that the QCL emits a comb for all the considered values of ΔLext\Delta L_{\mathrm{ext}}, as depicted in Fig. S.4.

Refer to caption
Figure S.4: Fine tuning of the EC cavity length LextL_{\mathrm{ext}} in the long cavity regime for a feedback-induced OFC. Temporal evolution of the power for different values of Lext=Lext,0+nλ/4L_{\mathrm{ext}}=L_{\mathrm{ext,0}}+n\lambda/4, with n=1,2,3,4=1,2,3,4. Lext,0=30L_{\mathrm{ext,0}}=30~{}cm, ϵ2=1%\epsilon^{2}=1~{}\%, I=1.08IthrI=1.08I_{\mathrm{thr}}, other parameters as in Table 1.

We can notice that also in this case the phase shift affects the waveform, but the type of dynamical regime (a comb in this case) is still the same for all the simulations. We have repeated this numerical experiment and verified the occurrence of this behaviour for other combinations of parameters, such as Lext,0=20L_{\mathrm{ext,0}}=20~{}cm, ϵ2=4%\epsilon^{2}=4~{}\% and Lext,0=20L_{\mathrm{ext,0}}=20~{}cm, ϵ2=1%\epsilon^{2}=1~{}\%, where comb emission is obtained for all the considered values of external cavity length shift ΔLext=nλ/4\Delta L_{\mathrm{ext}}=n\lambda/4, with n=1,2,3,4=1,2,3,4; for the combinations ofLext,0=40L_{\mathrm{ext,0}}=40~{}cm, ϵ2=4%\epsilon^{2}=4~{}\%, Lext,0=1L_{\mathrm{ext,0}}=1~{}m, ϵ2=36%\epsilon^{2}=36~{}\%, mixed state emission is obtained for all the considered values of external cavity length ΔLext=nλ/4\Delta L_{\mathrm{ext}}=n\lambda/4. Therefore, for the case I=1.08IthrI=1.08I_{\mathrm{thr}} (free-running CW as initial condition) these results show that in the short cavity regime an alternance between comb states and single mode emission occurs by performing a fine tuning of the external cavity on the λ\lambda scale. On the contrary, if we consider the long cavity regime, a variation in the length of the external cavity on the wavelength scale does not alter the type of dynamic regime emitted by the laser, although it implies a slight variation in the obtained waveform.

S.4 Estimation of the critical value of α\alpha factor for irregular dynamics

Refer to caption
Figure S.5: OFC indicators MσPM_{\sigma_{P}} and MΔΦM_{\Delta\Phi} as a function of the α\alpha factor, for Lext=1L_{\mathrm{ext}}=1 cm, ϵ2=36%\epsilon^{2}=36~{}\%, τe=5\tau_{\mathrm{e}}=5 ps, and other parameters as in Table I.
Refer to caption
Figure S.6: Example of irregular regime for α=0.5\alpha=0.5, τe=5\tau_{\mathrm{e}}=5 ps, Lext=1L_{\mathrm{ext}}=1 cm, ϵ2=36%\epsilon^{2}=36~{}\%, and other parameters as in Table I. (a) Temporal evolution of the output power. (b) Zoom on the first beatnote in the Power spectrum.

We estimated the critical value of α\alpha for which irregular dynamics is observed, considering the case Lext=1L_{\mathrm{ext}}=1 cm, ϵ2=36%\epsilon^{2}=36~{}\%, τe=5\tau_{\mathrm{e}}=5 ps, and simulating the QCL dynamics for the values of α\alpha between -0.1 and 0.7, with a step 0.1, and the other parameters fixed as in Table I. We chose this case because for α=0.1\alpha=-0.1 we have a comb regime, while for α=0.7\alpha=0.7 we report irregular dynamics, so that we are interested to estimate the value where the transitions between these two types of regimes occur. For a rigorous estimation, we calculate the comb indicators MσPM_{\sigma_{P}} and MΔΦM_{\Delta\Phi}. In Fig. S.5 we show the plot of the OFC indicators for different values of α\alpha for the mentioned case, and we observe a clear transition from comb to unlocked dynamics for α=0.5\alpha=0.5, a value which is compatible with THz QCLs.SilvestriReview; PiccardoReview We verified that the unlocked states reported for α0.5\alpha\geq 0.5 are actual irregular regimes and not mixed states (which are also unlocked according to the definition of the indicators, even if they present regular amplitude modulations with the periodicity given by the EC roundtrip). We remark that we referred to these states as "irregular" rather than "chaotic", because we did not assess their level of chaos using methods such as analyzing Lyapunov exponents, which would be necessary for accurately labeling them as "chaotic".
An example of these regimes, corresponding to α=0.5\alpha=0.5, is reported in Fig. S.6. It can be observed that the output power exhibits irregular modulations (Fig. S.6(a)), which do no present the periodicity given by the roundtrip of the external cavity. For this reason, they can not be classified as mixed states. If we look at the zoom on the first beatnote in the power spectrum (Fig. S.6(b)), we notice that this is split in several equidistant peaks spaced by the difference between FSR and FSRext\mathrm{FSR_{ext}}. In this case the nominal value of FSR is 20.820.8~{}GHz, FSRext=15\mathrm{FSR_{ext}}=15~{}GHz, and the found spacing in Fig. S.6(b) is 5.85.8~{}GHz. This shows that these irregular states arise from the beating between the external and laser cavity modes. By looking at the maps of Figs. 4(c)-(d) in the manuscript, we notice that they occur in a region where the FSR and FSRext\mathrm{FSR_{ext}} have the same order of magnitude. We understand, therefore, that in presence of high value of both α\alpha and feedback strength, if FSR and FSRext\mathrm{FSR_{ext}} have the same order magnitude we do not obtain a comb emission but an unlocked dynamics as described.

S.5 Fine Tuning of the external cavity length for a pre-existing frequency combs (OFC as initial condition)

Refer to caption
Figure S.7: Fine tuning of external cavity length in the short cavity regime, starting from a free-running comb emission (I=1.5IthrI=1.5I_{\mathrm{thr}}). Temporal evolution of the output power (left) and power spectrum (right) for different values of the EC length shift ΔLext\Delta L_{\mathrm{ext}}: (a) 0, (b) λ/4\lambda/4, (c) λ/2\lambda/2, (d) 3λ/43\lambda/4, (e) λ\lambda. λ\lambda is the central emission wavelength. Lext=7L_{\mathrm{ext}}=7~{}mm, ϵ2=1%\epsilon^{2}=1~{}\%, α=\alpha= -0.1; (b) τe=\tau_{\mathrm{e}}= 5 ps, other parameters as in Table 1.

We consider I=1.5IthrI=1.5I_{\mathrm{thr}}, corresponding to a free running comb emission. We add the feedback and, for some pairs (LextL_{\mathrm{ext}}, ϵ2\epsilon^{2}) we observe still emission of an OFC, as depicted in the map of Fig. 5(a) in the main manuscript (see the light blue region). Let us consider a pair in the light blue region, i.e. Lext=7L_{\mathrm{ext}}=7~{}mm, ϵ2=1%\epsilon^{2}=1~{}\%, which is also one of the cases displayed in Fig. 5(b) of the main manuscript. We perform a fine tuning of the EC length on the wavelength scale for this comb solution, reporting some differences with respect to the I=1.08IthrI=1.08I_{\mathrm{thr}} case discussed in Sec. S.3. In fact, we observe a passage from a comb regime (Fig. S.7(a)) to irregular dynamics (Fig. S.7(b)) when the EC length shift ΔLext\Delta L_{\mathrm{ext}} increases from 0 to λ/4\lambda/4, and then a return to comb for ΔLext=λ/2\Delta L_{\mathrm{ext}}=\lambda/2 (Fig. S.7(c)). Then, we again obtain irregular dynamics for ΔLext=3λ/4\Delta L_{\mathrm{ext}}=3\lambda/4, and a comb for ΔLext=λ\Delta L_{\mathrm{ext}}=\lambda. Therefore, our numerical simulations show that the comb solutions are obtained with periodicity λ/2\lambda/2.
If we consider a a case in the long cavity regime (Lext=60L_{\mathrm{ext}}=60~{}cm, ϵ2=1%\epsilon^{2}=1~{}\%), we observe that the comb states alternate with mixed states, characterized by a multi-peaked beatnote, as shown in Fig. S.8

Refer to caption
Figure S.8: Fine tuning of external cavity length in the long cavity regime, starting from a free-running comb emission (I=1.5IthrI=1.5I_{\mathrm{thr}}). Temporal evolution of the output power (left) and power spectrum (right) for different values of the EC length shift ΔLext\Delta L_{\mathrm{ext}}: (a) 0, (b) λ/4\lambda/4, (c) λ/2\lambda/2, (d) 3λ/43\lambda/4, (e) λ\lambda. λ\lambda is the central emission wavelength. Lext=60L_{\mathrm{ext}}=60~{}cm, ϵ2=1%\epsilon^{2}=1~{}\%, α=\alpha= -0.1; (b) τe=\tau_{\mathrm{e}}= 5 ps, other parameters as in Table 1.

This scenario is the result of the nonlinear competition between the EC and laser cavity modes in the QCL medium. These results reproduce the experimental findings presented in ref.Liao22, testifying the reliability of our simulator.

S.6 Feedback regime map for a mid-IR QCL

Homogeneous gain bandwidth δhom=1.1\delta_{\mathrm{hom}}=1.1 THz
Linewidth enhancement factor α=0.7\alpha=0.7
Central emission frequency ν0=30\nu_{0}=30~{}THz
Carrier lifetime τe=1\tau_{\mathrm{e}}=1~{}ps
Table 2: Model parameters for the simulation of a mid-IR QCL.SilvestriReview; Silvestri20; PiccardoReview; Faist_2016; Faist_book

In this section we replicate the study of Sec. III in the main manuscript for the case of a mid-IR QCL. We consider values of δhom\delta_{\mathrm{hom}}, α\alpha factor, central emission frequency ν0\nu_{0}, and carrier lifetime τe\tau_{\mathrm{e}} that are typical of mid-IR QCLs, as indicated in Table 2. For the ESMBE parameters not specified in Table 2 we utilize the values provided in Table 1. The value bias current value is I=1.08IthrI=1.08~{}I_{\mathrm{thr}}, and corresponds to single mode emission in free-running operation, in analogy with the study presented in Fig. 2 in the main manuscript.
The feedback diagram is shown in Fig. S.9.

Refer to caption
Figure S.9: Feedback regime diagram for a mid-IR QCL. The values of ϵ\epsilon and LextL_{\mathrm{ext}} are chosen in the same intervals as in the feedback maps of Figs. 2 in the main manuscript. The bias current of the QCL is I=1.08IthrI=1.08~{}I_{\mathrm{thr}}, and corresponds to single mode emission in free-running operation.

The higher value of gain bandwidth and α\alpha with respect to the THz QCL case of Fig. 2 leads to a larger number of modes involved in the competition inside the active medium. In fact, the phase-amplitude coupling provided by α\alpha favors the multimode dynamics of the laser,SilvestriReview; Opacak2019; Silvestri20 which can also manifest itself more easily in presence of a larger gain profile. For this reason, the dynamical scenario presented in the feedback map of Fig. S.9 is characterized by a large number of multimode states, both locked and unlocked. A comb region is observed for 4%<ϵ2<10%4~{}\%<\epsilon^{2}<10~{}\% in the short cavity range (Lext<1L_{\mathrm{ext}}<1~{}cm). However, for ϵ2>10%\epsilon^{2}>10\% we report a majority of irregular regimes if Lext<10L_{\mathrm{ext}}<10~{}cm. The high level of feedback, in combination with a larger α\alpha and more modes involved, implies an enhanced competition between external and laser cavity modes, and prevents the locking of the involved optical lines. Then, for Lext>10L_{\mathrm{ext}}>10~{}cm we observe mixed states, in analogy with the THz QCL diagram of Fig. 2.
Furthermore, we notice that the parameter configuration discussed in this section differs from the case of Fig. 4(c) in the main manuscript for the larger value of δhom\delta_{\mathrm{hom}}. This allows us to highlight the role of the gain bandwidth in the comb/multimode state formation in presence of an external target. In fact by comparing the two maps of Fig. S.9 and Fig. 4(c), we clearly observe that a larger gain bandwidth is crucial in order to have multimode regimes and comb formation in the short cavity range, and compensates the effect of the short carrier lifetime, which tends to keep stable the single-mode emission.mezzapesa2013; columbo2014

Refer to caption
Figure S.10: Temporal evolution of the output power for feedback-induced HFCs in mid-IR QCLs, with harmonic order 5 (a), 6 (b) and 7 (c). They are obtained for the same feedback ratio ϵ2=36%\epsilon^{2}=36~{}\% and for LextL_{\mathrm{ext}} respectively of 33~{}mm, 66~{}mm, and 22~{}mm. These combs are extracted from the map of Fig. S.9.

Finally, we observe that in the mid-IR QCL case, we report HFCs with order 5 (Fig. S.10(a)), 6 (Fig. S.10(b)), and 7 (Fig. S.10(c)), that were not found with the parameters of a THz QCL (in that case the maximum reported order was 4). This shows that in correspondence of lower values of both polarization dephasing time τd\tau_{\mathrm{d}} and carrier lifetime τe\tau_{\mathrm{e}} (and therefore faster carrier and polarization dynamics), HFCs characterized by a faster time scale can be generated in presence of feedback.