The ability to engineer quantum-cascade-lasers (QCLs) with ultrabroad gain spectra, and with a full compensation of the group velocity dispersion, at terahertz (THz) frequencies, is key for devising monolithic and miniaturized optical frequency-comb-synthesizers (FCSs) in the far-infrared. In THz QCLs four-wave mixing, driven by intrinsic third-order susceptibility of the intersubband gain medium, self-locks the optical modes in phase, allowing stable comb operation, albeit over a restricted dynamic range (∼20% of the laser operational range). Here, we engineer miniaturized THz FCSs, comprising a heterogeneous THz QCL, integrated with a tightly coupled, on-chip, solution-processed, graphene saturable-absorber reflector that preserves phase-coherence between lasing modes, even when four-wave mixing no longer provides dispersion compensation. This enables a high-power (8 mW) FCS with over 90 optical modes, through 55% of the laser operational range. We also achieve stable injection-locking, paving the way to a number of key applications, including high-precision tunable broadband-spectroscopy and quantum-metrology.
The ability to engineer quantum-cascade-lasers (QCLs) with ultrabroad gain spectra, and with a full compensation of the group velocity dispersion, at terahertz (THz) frequencies, is key for devising monolithic and miniaturized optical frequency-comb-synthesizers (FCSs) in the far-infrared. In THz QCLs four-wave mixing, driven by intrinsic third-order susceptibility of the intersubband gain medium, self-locks the optical modes in phase, allowing stable comb operation, albeit over a restricted dynamic range (∼20% of the laser operational range). Here, we engineer miniaturized THz FCSs, comprising a heterogeneous THz QCL, integrated with a tightly coupled, on-chip, solution-processed, graphene saturable-absorber reflector that preserves phase-coherence between lasing modes, even when four-wave mixing no longer provides dispersion compensation. This enables a high-power (8 mW) FCS with over 90 optical modes, through 55% of the laser operational range. We also achieve stable injection-locking, paving the way to a number of key applications, including high-precision tunable broadband-spectroscopy and quantum-metrology.
Optical frequency
comb synthesizers
(FCSs) enable broadband coherent light sources to be developed, comprising
a large number of equally spaced lasing modes.[1] Chip-scale, broadband, monolithic, high brightness FCS sources at
THz frequencies are needed for metrology,[2−6] ultrahigh speed communications,[6] coherent nanotomography,[7] and
near-field broadband nanoscopy and enable new approaches to high-resolution
broadband molecular spectroscopy, manipulation of complex molecules
and cold atoms, astronomy, and attosecond science.[8]QCLs are the highest brightness miniaturized sources
in the infrared
(IR).[9,10] They combine an inherently high spectral
purity,[11,12] with a very broad bandwidth,[13−15] Watt-level output-powers,[16] and a long
upper-state lifetime (>5–10 ps). Broad emission in the THz
range can be attained by quantum-tailoring the gain medium to host
heterogeneous stacks of individual active regions, which themselves
are incorporated into a monolithic microstrip-line metal–metal
resonator.[17,18] The cascading design of individual
emitters at complementary wavelengths creates a flat broad-gain at
a desired bias point, which is usually slightly above the onset of
multimode emission. The long upper state lifetime (≥5–10
ps)[9,10,19] of THz QCLs
inhibits mode-locking but favors phase-matching between the cavity
modes driven by the ultrafast nonlinearity (four-wave mixing, FWM)
spontaneously arising in the intersubband gain medium.[13,15,20] The resulting stable frequency
comb regime tends, however, to be restricted to lower injection currents,
close to the onset of multimode emission, owing to the intersubband
bias-dependent contribution to the group velocity dispersion.[13,15,20] The heterogeneous nature of the
gain media then entangles the dispersion dynamics at other biases.[20] Tailoring the dynamic (bias-dependent) contribution
to the chromatic dispersion is, therefore, crucial for establishing
perfectly spaced, phase-locked, high-intensity modes spanning the
entire dynamic range of the laser.The use of chirped mirrors[20] and/or
coupled cavities[21−23] was proposed for group velocity dispersion (GVD)
compensation in homogeneous[20,21] and heterogeneous[22,23] THz QCL FCSs, respectively. In the first case, the corrugation length
and the tapering period of a chirped cavity was designed to optimize
the anomalous group delay dispersion (GDD) in a specific, narrow,
range of biases, leading to an FCS extending over 24% of the laser
dynamic range, covering a 0.6 THz spectral bandwidth, but with an
uneven distribution of power among the 60 modes.[20] In the second case, a coupled cavity, mimicking a Gires–Tournois
interferometer (GTI),[21] was monolithically
integrated in front of the THz QCL cavity, introducing chromatic dispersion
that compensates for that in the gain medium.[21] When DC biased, the small coupled-cavity section gave rise to an
FCS over the whole QCL dynamic range, although there was only a very
limited amount of optical power (μW) over <0.4 THz bandwidth,
allocated among a few, irregularly distributed modes of dissimilar
intensities. This was a result of dual-cavity induced suppression
of the multimode operation regime.[21] Such
coupled cavity architectures are extremely beneficial for generating
ultrashort THz pulses through injection seeding.[22] Using a very small intracavity spacing (1.5–2 μm),
and predefined coupled-cavity lengths, effective chromatic dispersion
compensation was achieved. However, this was only possible over a
very limited frequency range, due to the nonlinear phase-frequency
relation associated with the dispersion. Oscillation in the group
delay dispersion (GDD) was expected, as the phase of the reflected
light, and GDD, change periodically with the optical frequency, owing
to resonance effects.[22]Despite these
advances, there remains a lack of miniaturized technologies
for high-power (>5 mW), broadband (∼1 THz bandwidth) THz
QCL
FCSs, providing phase-locked, evenly spaced, lines of comparable intensity
over the entire laser dynamic range. Furthermore, for high-precision
(10–11) and high-sensitivity (one part in 10–6 cm–1/Hz–1/2)
metrological applications, there
is a further requirement for fine frequency tunability of the comb
lines over a broad spectral window, combined with an (ideally) zero
time jitter of the phase-locked modes, and small phase fluctuations.
This would allow THz QCL FCSs to be fully stabilized against primary
frequency standards.[24]Here, we present
a record dynamic range THz QCL FCS based on a
monolithic coupled-cavity architecture, comprising a heterogeneous
THz-frequency QCL, with a wide (3.2) dynamic range, and an on-chip
solution-processed multilayer graphene saturable absorber (GSA) reflector,
and demonstrate stable injection locking. The gapless nature of graphene,
and the related frequency-independent absorption, ultrafast recovery
time,[25] low saturation fluence,[26] and ease of fabrication[27] and integration,[28,29] makes it an appealing nonlinear
optical component in the infrared, and ideal for developing THz QCL
FCSs, with performances far-beyond any alternative technology developed
so far. Furthermore, graphene can be employed to introduce intensity
dependent losses into the external laser cavity.[30,31] To date, graphene has been employed as external element, in transmission,
to induce changes in the emission spectra of a THz QCL emitting over
a limited (0.15 THz) spectral window.[32]Here, we use a heterogeneous 17-μm-thick GaAs/AlGaAs
heterostructure
comprising three active modules, with gain bandwidths centered at
2.5, 3, and 3.5 THz and comparable threshold current densities (Jth). This leads to a very broad operational
dynamic range of the heterogeneous gain medium: Jdr = Jmax/Jth = 3.2, where Jmax is the
maximum working current density.[15,17] Sample fabrication
is based on a metal–metal processing technique, with lossy
side absorbers lithographically implemented along the waveguide edges,
as discussed in Methods.[15,33] The resulting lasers work as fully stabilized optical frequency
comb synthesizers over 16% of their dynamic range,[15] as we recently demonstrated through the full-control and
stabilization of the characteristic FCS parameters, i.e., the separation
between adjacent modes and the carrier offset frequency, measured
using a multiheterodyne detection scheme, in which the QCL-comb was
mixed with a fully stabilized optically rectified THz-frequency comb.[24]The graphene reflector is prepared by
liquid phase exfoliation
(LPE) of graphite in a water/surfactant solution (see Methods).[30] The resulting film
is ∼65 nm thick, as determined by atomic force microscopy[30] and covers a surface of about 1 cm2. Raman spectroscopy is used to monitor the quality of the flakes
at each step of the preparation process as well as to qualitatively
estimate, in combination with electrical transport tests, the Fermi
energy, EF ≤ 250 meV.[30] The resultant reflector (58% reflectivity in
the THz)[30] behaves as an intraband driven
(fast) saturable absorber at THz frequencies, providing 80% transparency
modulation, as a result of the intraband induced absorption bleaching.[30] This is confirmed when using our fully stabilized
optical frequency comb in pulsed mode (10% duty cycle) (see Supporting Information and Supplementary Figure S1).The graphene reflector is
then mounted on a Cu mount, via a thin
indium foil (see Figure a), to ensure optimal thermal contact with the QCL Cu mount, with
which it is in close thermal contact.
Figure 1
THz QCL with an on-chip graphene saturable
absorber (GSA) reflector.
(a) Schematic of a THz QCL comb coupled on chip with a GSA reflector;
(b) Continuous-wave (CW) current–voltage (I–V) and light-current
(L–I) characteristics of a 3.6 mm long, 50 μm wide THz
QCL at a heat sink temperature of 15 K, without (R) and with (G) the on-chip GSA reflector. The optical
power is measured with a calibrated power-meter (Thomas Keating Ltd.)
and corrected to take into account the 75% absorption of the cryostat
window. The light blue shaded areas correspond to the regimes in which
the laser behaves like an optical frequency comb synthesizer.
THz QCL with an on-chip graphene saturable
absorber (GSA) reflector.
(a) Schematic of a THz QCL comb coupled on chip with a GSA reflector;
(b) Continuous-wave (CW) current–voltage (I–V) and light-current
(L–I) characteristics of a 3.6 mm long, 50 μm wide THz
QCL at a heat sink temperature of 15 K, without (R) and with (G) the on-chip GSA reflector. The optical
power is measured with a calibrated power-meter (Thomas Keating Ltd.)
and corrected to take into account the 75% absorption of the cryostat
window. The light blue shaded areas correspond to the regimes in which
the laser behaves like an optical frequency comb synthesizer.The graphene reflector is coupled on-chip, perpendicular
to the
back facet of a 3.6-mm-long, 50-μm-wide heterogeneous THz QCL,
with a separation of 15 μm, meaning that it can be approximated
as part of the laser cavity, and finely aligned by means of calibrated
screws. A picture of the GSA reflector is shown in the bottom part
of Figure a. The unbiased
reflector and the QCL, forming a coupled cavity with a 15 μm
air gap (GTI), are then mounted onto the coldfinger of a continuous-flow
He cryostat. Light emission (Figure b) is measured from the QCL using the facet opposite
to the graphene reflector, as illustrated in the graphics of Figure a. This chip-scale
embedded integration of the GSA ensures long-term stability, appropriate
thermal management, and reproducibility of the experimental results.In this configuration, the Gires Tournois interferometer does not
affect the total QCL GDD, as shown by numerical simulations of the
dispersion compensation performed using a finite element method (Comsol
Multiphysics) (see Methods), Figure a–c.
Figure 2
(a) Individual simulated
group delay dispersion (GDD) of the GTI
composed by GSA reflector, the QCL comb material and gain GDD, the
total GDD for the specific GTI length of 15 μm. (b) Individual
simulated GDD of the GTI composed of the 420 μm thick SiO2/Si substrate, the QCL comb material and gain GDD, the total
GDD for a GTI length of 15 μm. (c) Individual simulated GDD
of the GTI composed by the GSA reflector, the QCL comb material and
gain GDD, the total GDD for the specific GTI length of 55 μm,
i.e., for an “on-resonance GTI”.
(a) Individual simulated
group delay dispersion (GDD) of the GTI
composed by GSA reflector, the QCL comb material and gain GDD, the
total GDD for the specific GTI length of 15 μm. (b) Individual
simulated GDD of the GTI composed of the 420 μm thick SiO2/Si substrate, the QCL comb material and gain GDD, the total
GDD for a GTI length of 15 μm. (c) Individual simulated GDD
of the GTI composed by the GSA reflector, the QCL comb material and
gain GDD, the total GDD for the specific GTI length of 55 μm,
i.e., for an “on-resonance GTI”.At a distance of 15 μm, the total GDD does not show any significant
variation, either when the QCL is integrated with the GSA reflector
(Figure a), or when
it is combined with the bare 420 μm thick SiO2/Si
substrate (Figure b). This is expected, as the phase change introduced by the GTI is
almost negligible for such a small distance. Therefore, in this strong
coupling condition, it is expected that dispersion compensation does
not play any role in the phase-dynamics of the QCL comb modes, that
are, in practice, unperturbed by the GTI, as in the case when a SiO2/Si substrate is strongly coupled to the QCL. We then perform
the same simulations while matching the distance d with the first resonance of our GTI,[23] i.e., d = 55 μm (Figure c). Unlike what obtained with a coupled Aumetal mirror,[23] the GDD introduced by the
GTI is over 1 order of magnitude lower than that arising from the
QCL gain, meaning that no dispersion compensation is expected. We
consider this effect to be a result of the high absorption of the
graphene stack, which limits the feedback to the QCL.In the
following the GSA coupled-cavity laser is labeled as “G”,
with “R” referring to the same QCL with the on-chip
GSA reflector.Comparison between continuous-wave (CW) current–voltage
(I–V) and light–current (L–I) characteristics
(Figure b) of the
GSA coupled cavity laser (sample G) and of the bare, QCL (sample R)
shows that, while the device transport is not affected by the presence
of the coupled reflector, the optical power benefits from the nonlinear
reflector. An optical power of 8 mW is measured from the front facet
of sample G, a factor of 2 larger than that of the bare sample R.
Furthermore, the GSA reflector leads to factor ∼2.3 increase
in slope efficiency.Considering the ±40° divergence
(Supplementary Figure S2) measured from
our double-metalTHz
QCL comb, and since the power emitted from the back facet of the QCL
is initially equal to that measured from the reference sample R, the intensity of the THz beam impinging on the GSA reflector
varies from I0 ∼ 100 W/cm2 just above threshold (I = 400 mA) to I0 ∼ 800 W/cm2 at the optical peak power
(I = 835 mA), well above the saturation intensity
(Is ∼ 6.3–6.7 W/cm2) (ref (30) and Supporting Information) over the full dynamic
range of the laser, confirming that the graphene film behaves as a
saturable absorber.[30]Representative
CW Fourier transform infrared spectra (FTIR) under-vacuum
(Figure a–d),
measured for different currents in the G sample, show that well above
threshold (>880 mA) (Figure b–d) the GSA reflector does not induce major changes
in the spectral behavior of the laser (see Figure f–h for comparison with the R sample)
over most of its operational range. It activates some additional peaks
in the 2.3–2.4 THz region (Figure a–d) that persist over the whole operational
range, and that are absent in the bare laser (Figure e–h).
Figure 3
FTIR emission spectra collected under
vacuum with a Bruker (Vertex
80) spectrometer in rapid scan mode, with a 0.075 cm–1 resolution in the G sample (a–d) and in
the R sample (e–h). The QCL is operated in
CW at a fixed heat sink temperature = 15 K at driving currents of
(a,e) 560 mA, (b,f) 880 mA, (c,g) 950 mA, and (d,h) 1050 mA, respectively.
The dashed horizontal lines indicate the noise floor of the measurements.
FTIR emission spectra collected under
vacuum with a Bruker (Vertex
80) spectrometer in rapid scan mode, with a 0.075 cm–1 resolution in the G sample (a–d) and in
the R sample (e–h). The QCL is operated in
CW at a fixed heat sink temperature = 15 K at driving currents of
(a,e) 560 mA, (b,f) 880 mA, (c,g) 950 mA, and (d,h) 1050 mA, respectively.
The dashed horizontal lines indicate the noise floor of the measurements.A remarkable difference is detected at 560 mA (J = 311 A/cm2). The G sample spectrum in Figure a has families of
lasing modes
individually spaced by the cavity round trip time, but the families
are separated by a frequency matching a high order harmonic (9th)
of the cavity’s round trip frequency. Such a phenomenon is
typical of harmonic mode locking, happening when multiple pulses per
round trip are generated as a consequence of the modulation applied
at harmonics of the cavity’s fundamental round trip frequency.[34] The spectrum of the G sample then broadens gradually
with bias, reaching a continuous bandwidth of 0.94 THz (2.55–3.49
THz) at a current of 880 mA, and a discontinuous bandwidth of 1.25
THz (2.30–3.55 THz), with 8 mW of CW power, distributed among
90 equally spaced optical modes, as shown in Figure b.Figure a plots
the corresponding free running electrical beatnote map, typically
performed to characterize the coherence of the spectral emission of
QCL-based frequency combs.[13]
Figure 4
Analysis of
intermode beatnote. (a) Intermode beatnote map as a
function of QCL bias current for a 3.6 mm long, 50 μm wide laser
bar integrated on-chip with a GSA reflector. The beatnote signal is
extracted from the bias line with a bias-tee and recorded with an
RF spectrum analyzer (Rohde and Schwarz FSW; RBW: 500 Hz, video bandwidth
(VBW): 500 Hz, sweep time (SWT): 20 ms, RMS acquisition mode). All
measurements are performed in CW at a fixed heat sink temperature
= 15 K. The two star symbols indicate representative driving current
regimes (I = 456 mA) and (I = 928
mA) in which the device behaves like a stable frequency comb synthesizer.
(b,c) Intermode beatnote line width as a function of driving current
measured on (b) the GSA coupled QCL (G sample) and
(c) the bare laser (R sample); (d,e) Intermode beatnote
trace recorded at (c) I = 456 mA with center frequency
at 11.345 GHz, and (d) at I = 928 mA with center
frequency at 11.426 GHz, respectively.
Analysis of
intermode beatnote. (a) Intermode beatnote map as a
function of QCL bias current for a 3.6 mm long, 50 μm wide laser
bar integrated on-chip with a GSA reflector. The beatnote signal is
extracted from the bias line with a bias-tee and recorded with an
RF spectrum analyzer (Rohde and Schwarz FSW; RBW: 500 Hz, video bandwidth
(VBW): 500 Hz, sweep time (SWT): 20 ms, RMS acquisition mode). All
measurements are performed in CW at a fixed heat sink temperature
= 15 K. The two star symbols indicate representative driving current
regimes (I = 456 mA) and (I = 928
mA) in which the device behaves like a stable frequency comb synthesizer.
(b,c) Intermode beatnote line width as a function of driving current
measured on (b) the GSA coupled QCL (G sample) and
(c) the bare laser (R sample); (d,e) Intermode beatnote
trace recorded at (c) I = 456 mA with center frequency
at 11.345 GHz, and (d) at I = 928 mA with center
frequency at 11.426 GHz, respectively.Beatnote signals are extracted from the bias line, using a bias-tee,
and recorded with a radio frequency (RF) spectrum analyzer. A change
in the intermode beatnote signal map is seen for the whole operational
range of the QCL, when compared to that of the reference laser.[15,24] At J = 228 A/cm2, when band alignment
is fully reached, as typical of most QCL based frequency combs, the
optical modes of the reference laser (sample R) lose their phase coherence
and the intermode beatnote significantly broadens (>100 MHz line
width)
as the GVD becomes large enough to prevent FWM from locking the lasing
modes in frequency and phase simultaneously.[15,24] This contrasts with the bias-dependent evolution of the beatnote
map of the G sample (Figure a). The introduction of the GSA reflector causes a significant
enlargement (from 16% (Figure c, and ref (15)) to 55% of the laser operational range (Figure a)) of the dynamic range in which THz QCL
frequency comb is observed.The comparative analysis of the
beatnote line width (Figure b,c) discloses the efficacy
of our approach. A set of individual beatnotes, as narrow as 780 Hz
(Figure d), persists
in the current range between 350 and 480 mA, as shown in Figure b. The beatnote is
a factor of 5 narrower than measured in the reference sample,[24] (Figure c), at specific biases/currents, thus suggesting that the
GSA integration improves the phase locking of the optical modes. In
analogy with the bare laser (sample R),[15,24] in the region
between 350 and 480 mA, the RF beatnote signals are blue-shifted with
a coefficient 3.6 MHz/mA. This is a consequence of the changes in
the relative distance between the beating modes, induced by the chromatic
dispersion in the gain spectrum.When the current in sample
G is increased from 480 to 500 mA, the
single beatnote line width increases to 10 kHz, although it still
preserves its narrow nature (Figure b). Conversely, above 476 mA, the bare laser (sample
R) (Figure c)[15] looses its phase coherence[24] and develops a broad beatnote regime, reaching ∼300
MHz line width at 500 mA.In the current range 500–525
mA, the beatnote of sample
G remains single, but superimposed to a broader beatnote (100–880
kHz). Over a very small (10 mA) current range, around 570 mA, the
beatnote turns again single and narrow (950 Hz). This is a signature
that the dispersion compensation in sample G enables phase locking
of the emitted optical modes.In the 580–780 mA range,
the beatnote line width increases
to 200–500 MHz, signature of a transport regime dominated by
dispersion. However, a single beatnote is still visible, superimposed
on a broader signal (see Figure a). Although wider, the presence of such an individual
beatnote enables locking it to a microwave reference, in order to
mode-lock the QCL and, consequently, reduce the beatnote line width.[35]
Figure 5
(a) Stacked intermode beatnote traces recorded at a heat
sink temperature
= 15 K, while driving the GSA-coupled QCL (G) and the bare laser (R)
at J = 350 A/cm2. The spectrum analyzer
settings are RWB: 10 kHz, VBW: 100 kHz, and SWT: 500 ms. The line
width is limited by the RBW of the spectrum analyzer. (b) Intermode
beatnote line width as a function of driving current measured on the
bare laser, while coupling it with the 420 μm thick SiO2/Si substrate, placed at a distance of 15 μm from the
QCL back facet.
(a) Stacked intermode beatnote traces recorded at a heat
sink temperature
= 15 K, while driving the GSA-coupled QCL (G) and the bare laser (R)
at J = 350 A/cm2. The spectrum analyzer
settings are RWB: 10 kHz, VBW: 100 kHz, and SWT: 500 ms. The line
width is limited by the RBW of the spectrum analyzer. (b) Intermode
beatnote line width as a function of driving current measured on the
bare laser, while coupling it with the 420 μm thick SiO2/Si substrate, placed at a distance of 15 μm from the
QCL back facet.Similarly, in the 780–835
mA range, the beatnote remains
single but turns narrower and is superimposed on a broader one (100–790
kHz). In contrast, a fully dispersion dominated regime is observed
in sample R, over >80% of its dynamic range (Figure c),[15] i.e., for
all currents >536 mA.The most significant effect of the
GSA reflector appears at driving
currents >845 mA (i.e., for J = 2.6–3.2 Jth), where the single beatnote line width preserves
its narrow nature (600 Hz–10 kHz) (Figure b,e). This corresponds to the high-phase
noise regime typically recorded at larger current densities in the
bare laser (sample R), and in all other THz QCL combs, reported to
date, when J > 1.16 Jth.This single and narrow beatnote is in contrast to that detected
in the R sample, in which spontaneous FWM phenomena are typically
unable to support dispersion compensation.[13,15,20] The GSA reflector provides a clear advantage
with respect to any alternative saturable absorbers developed so far
at THz frequencies such as n-doped semiconductors (GaAs, GaP, and
Ge). Although these materials can be used as THz SAs, they require
electric fields of 10s kV/cm and cannot be easily integrated with
a THz QCL using an approach similar to that described here, without
inducing a major detrimental increase of the external cavity losses
due to free carrier absorption.By progressively driving the
laser toward the negative differential
resistance regime, the narrow beatnote red-shifts with a coefficient
−0.33 MHz/mA, mainly due to the local heating of the lattice
at higher driving currents.Figure d,e plots
the intermode beatnote spectra in the two most interesting transport
regimes in which in the QCL behave like a comb: 456 mA (Figure d) and 928 mA (Figure e). Beatnote line widths as
narrow as 780 Hz (Figure d) and 600 Hz (Figure e) can be seen the narrowest to date in any THz QCL FCS, to
the best of our knowledge. Correspondently, in the latter case, the
spectrum shows a 0.94 THz spectral coverage, with a high output power
(8 mW of CW power; 40 mW of peak power in pulsed mode, maximum wall
plug efficiency 0.1%), distributed among 90 equally spaced optical
modes. This sets the state of the art THz QCL frequency combs. It
is worth mentioning that the line width values are ultimately limited
by the jitter of the beat-note, since the laser is not stabilized.The explanation of the behavior at I > 845 mA is a consequence
of the mechanism through which the graphene-related dynamics contributes
to stabilize the QCL optical modes. Frequency and phase locking of
the modes, prerequisite of comb formation, can be obtained through
FWM generated by either fast saturable gain or loss in semiconductor
lasers.[36] The former mechanism leads to
a frequency modulated output, while the latter is associated with
amplitude modulation. In THz QCL FC, both frequency and amplitude
modulation are typically present,[37] and
act simultaneously. In our setup, the gain and absorption are spatially
separated, so they do not average out to a local net gain/loss, and
create a spatially dependent profile within the cavity. The above
arguments explain why, as a result of the interaction of the field
emitted by the QCL with the inherently fast GSA,[30] and the related reinjection of this field into the laser
cavity, the fast saturable loss of the GSA contributes to the locking
between the modes, which manifests itself by the observed extremely
narrowed beatnote.The dynamical processes behind the generation
of such a sharp and
narrow beatnote, following the above arguments, are then investigated
by performing time-domain simulations based on the Maxwell-Bloch equations
in the configuration in which the QCL is uncoupled (sample R) or tightly
coupled (sample G) with the GSA. We use the mbsolve[38] software, which is an open-source solver for the one-dimensional
Maxwell-Bloch equations capable of handling spatial regions of different
materials. We investigate the dynamical behavior of our experimental
system, as described in the Supporting Information. The QCL is modeled as two-level gain medium, with the physical
parameters summarized in Table I (Supporting Information). Subsequently, we derive the intermode beatnote spectrum from the
optical field, for both cases. The simulation results (Figure S3), in agreement with our experimental
findings, show a reduction of the intermode beatnote line width when
the QCL is integrated with the GSA.In addition to the saturable
absorption effect inside graphene,
the reflector also features Fresnel reflection on the graphene surface.
Since this component is spatially separated from the saturable absorption
occurring inside graphene, it might contribute to frequency comb stabilization
through the same mechanism as the fast saturable gain in the active
region. These effects then try to force the QCL into frequency-modulated
operation, while the saturable absorption in graphene helps regularize
the remaining amplitude modulations.The combination of the
above effects can explain our experimental
observations.To further confirm our arguments, we perform a
further set of experiments.First, Figure b
compares the reference unperturbed QCL beatnote evolution with the
corresponding beatnote line width evolution recorded when the 420-μm-thick
Si/SiO2 substrate is coupled (at 15 μm distance)
to one end of the QCL laser cavity, in the same position of the GSA
reflector. No difference is seen in the beatnote map with respect
to the bare laser, confirming that the dispersion compensation, arising
from the Si/SiO2 50% reflector, as predicted by numerical
simulations (Figure a,b), does not play a role, and the GSA reflector is driving the
intermode dynamics.Second, we perform two set of experiments
in which we collect the
intermode beatnote line widths by varying the distance of both GSA
and Si/SiO2 from the end of the QCL laser cavity (d), respectively, while keeping the current at I = 900 mA, i.e., in the region in which the most significant differences
are unveiled.In both cases, we first vary d finely in the 15–25
μm range, then in the range 25–200 μm with the
impinging laser beam intensity I ≤ Is, and then in the range 200–500 μm,
where I ≪ Is.
The rationale is that, since GTIs are extremely sensitive to the distance
from the laser facet, any change of the beatnote map would be a signature
of a GDD compensation operated by the GTI. The analysis of the intermode
beatnote line width (Figure a,b) at 900 mA, shows that in our G sample, by varying d in and out resonance, the intermode beatnote remains single
and preserves its narrow nature (Figure a) for d ≤ 200 μm,
unlike what experimentally observed in the case of a dispersion compensated
GTI THz QCL comb,[23] achieved by coupling
a metal mirror.
Figure 6
(a,b) Evolution of electrical intermode beatnote line
width of
GSA-coupled QCL as a function of the distance d of the GSA from the
laser facet, for a fixed driving current of 900 mA. (c) Evolution
of the electrical intermode beatnote line width of the QCL coupled
with a 420-μm-thick SiO2/Si substrate, as a function
of the distance d of the SiO2/Si substrate from the laser
facet, for a fixed driving current of 900 mA. All measurements are
performed in CW at 15 K. The beat-note signal is extracted from a
bias line, employing a bias-tee connected to a RF optical spectrum
analyzer (OSA) in RMS acquisition mode (OSA setting: RWB: 500 Hz,
VBW: 500 Hz, SWT: 50 ms).
(a,b) Evolution of electrical intermode beatnote line
width of
GSA-coupled QCL as a function of the distance d of the GSA from the
laser facet, for a fixed driving current of 900 mA. (c) Evolution
of the electrical intermode beatnote line width of the QCL coupled
with a 420-μm-thick SiO2/Si substrate, as a function
of the distance d of the SiO2/Si substrate from the laser
facet, for a fixed driving current of 900 mA. All measurements are
performed in CW at 15 K. The beat-note signal is extracted from a
bias line, employing a bias-tee connected to a RF optical spectrum
analyzer (OSA) in RMS acquisition mode (OSA setting: RWB: 500 Hz,
VBW: 500 Hz, SWT: 50 ms).In the latter case, a narrow (∼3 kHz) and intense beatnote
is only achieved at periodic positions of the external metal coupling
element.[23] For d >
205
μm (Figure b),
the GSA-integrated QCL behavior is identical to that of the bare laser,
a signature that the GSA plays no role. As expected, in the Si/SiO2-coupled QCL, the distance does not affect the broad line
width (>100 MHz), which persists over the whole range of distances
(Figure c).The ability to coherently frequency stabilize the GSA reflector
is further proved by applying a direct RF modulation at its round-trip
frequency. Injection of a periodic signal into an oscillator is commonly
used to stabilize emission frequency and/or laser cavity modes separation,[39] and corresponds to round-trip frequency stabilization,
as normally achieved by injection of an external microwave signal
on the driving current. Reference (35) demonstrated injection locking of the intermode
frequency difference of THz QCL over hundreds of MHz by driving the
laser bias with a microwave signal close to this frequency. Reference (40) achieved the stabilization
of the frequency difference between two lateral modes of a THz QCL
with corresponding frequency locked line widths ≤10 Hz and
with a negligible drift. Here, we demonstrate the stability of our
GSA-coupled QCL-comb intermode separation by measuring the shape of
its photocurrent spectrum in the microwave range, around the cavity
round-trip frequency, where a sharp single peak proves stable phase
and frequency relation between adjacent laser modes.Figure a,b shows
all-electrical injection locking of a narrow beatnote to the RF oscillator,
and the corresponding locking range, as a function of the RF-power
transmitted inside the cavity of sample G. This follows
the square root behavior predicted by Adler’s equation.[35]
Figure 7
Coherent injection locking. (a,b) Locking range as a function
of
RF-power transmitted inside the cavity of a THz QCL-comb integrated
on-chip with a GSA reflector. The RF and dc-bias signals are brought
to the QCL using a 60 GHz, 50 Ω coplanar probe positioned at
one end of the QCL ridge. The intermodal beatnote (IBN) frequency
is at a repetition frequency ∼11 GHz, and is electrically extracted
from the QCL by connecting the RF-synthesizer to the input port of
a 40 GHz directional coupler, with the output port of the coupler
connected to the ac input of a 40 GHz bias-Tee. The dc line of the
bias-Tee is connected to the power supply that drives the QCL at a
constant current of (a) 425 mA, and (b) 980 mA. The spectra are collected
with the same settings of Figure a. (c,d) IBN spectra for different RF injected powers.
The RF frequency is held constant at approximately (c) 6 MHz or (d)
0.4 MHz apart from the cavity round trip frequency, and the laser
is operating at (c) 425 mA, and (d) 980 mA. Microwave spectra are
on a logarithmic scale for different injected powers.
Coherent injection locking. (a,b) Locking range as a function
of
RF-power transmitted inside the cavity of a THz QCL-comb integrated
on-chip with a GSA reflector. The RF and dc-bias signals are brought
to the QCL using a 60 GHz, 50 Ω coplanar probe positioned at
one end of the QCL ridge. The intermodal beatnote (IBN) frequency
is at a repetition frequency ∼11 GHz, and is electrically extracted
from the QCL by connecting the RF-synthesizer to the input port of
a 40 GHz directional coupler, with the output port of the coupler
connected to the ac input of a 40 GHz bias-Tee. The dc line of the
bias-Tee is connected to the power supply that drives the QCL at a
constant current of (a) 425 mA, and (b) 980 mA. The spectra are collected
with the same settings of Figure a. (c,d) IBN spectra for different RF injected powers.
The RF frequency is held constant at approximately (c) 6 MHz or (d)
0.4 MHz apart from the cavity round trip frequency, and the laser
is operating at (c) 425 mA, and (d) 980 mA. Microwave spectra are
on a logarithmic scale for different injected powers.The RF-signals capture the comb oscillator, imposing an oscillation
frequency even when the RF power is as low as −29 dBm (Figure a, I = 400 mA), provided that the two oscillators are at sufficiently
close frequencies and their coupling is strong enough. Equally, with
a higher laser current (Figure b, 980 mA), locking is observed, albeit with higher injection
power levels.[39]To investigate the
injection locking dynamics further, we retrieve
the beat note spectra, measured in the single beatnote regimes, as
the injected RF power is increased. The broad beatnote is pulled toward
the frequency of the injected signal (11.2200 GHz, Figure c; 11.4164 GHz, Figure d) and finally locked, as shown
in Figure c,d at the
different bias currents of 425 mA (Figure c) and 980 mA (Figure d), respectively. Two side peaks ∼9
dBm weaker than the initial beatnote remain for RF injected powers
up to −8 dBm in Figure c, then vanish, and the microwave spectrum of the intermode
beating is fully controlled by the injected signal. The noise floor
around the locked narrow beatnote is ∼20 dB, i.e., weaker than
the peak power of the originally broad beatnote. This proves that
the intermode beatnote power is almost completely locked.In
conclusion, we demonstrated that the free-running phase coherence
of broadband THz QCLs with a heterogeneous active region can be enhanced
by on-chip coupling to a saturable absorber prepared from a liquid
phase exfoliated graphite film. With the on-chip integration of a
GSA reflector on a fully stabilized THz comb, operating only over
16% of its dynamic range,[24,15] we achieve stable comb
operation through 55% of the laser operational range, with a beatnote
line width as narrow as 600 Hz, 8 mW of CW power and 90 equally spaced
optical modes covering a 0.94 THz spectral bandwidth, with more than
three-decade reduction of phase-noise over an additional 15% of this
range. We also achieve injection locking over the same operational
range as the FCS, showing the stability of the comb operation. Our
compact and frequency agile design, together with the high optical
power, the large number of optical modes, and the narrow beatnote
line width, well suited for dual-comb THz spectroscopy[41] and hyperspectral imaging,[42] paves the way to deliver an all-in-one miniaturized nanoengineered
frequency comb electrical sources for spectroscopic and nanoscale
applications in the far-infrared. Our design, in conjunction with
graphene’s fast recovery time and saturation fluence, could
produce time domain pulses with sub-ps widths and average power comparable
to the CW operation level of a QCL.
Methods
QCL Fabrication
Lasers are fabricated in a metal–metal
waveguide configuration. We first perform Au–Au thermo-compression
wafer bonding of the 17-μm-thick active region (sample L1458)
onto a highly doped GaAs substrate, followed by the removal, through
a combination of mechanical lapping and wet etching, of the host GaAs
substrate of the molecular beam epitaxial (MBE) material. The Al0.5Ga0.5As etch stop layer is removed using HF etching.
Laser bars are then defined by inductively coupled plasma etching,
which leads to almost vertical sidewalls (hence uniform current injection
into the full gain region). Following etching, a Cr/Au (10 μm/150
μm) top contact is deposited along the center of the ridge surface,
leaving a thin region uncovered along the ridge edges. The 5 μm-wide
Ni (5-nm-thick) side absorbers are then deposited over the uncovered
region, using a combination of optical lithography and thermal evaporation.
Such lossy side absorbers are intended to inhibit lasing of the higher
order lateral modes by increasing their threshold gain.[5] Finally, the backside of the substrate is lapped
down to 150 μm to optimize thermal management and enable operation
in CW. Laser bars, 50 μm wide and 3.6 mm long, are then cleaved
and mounted on a Au-coated Cu bar, and then onto the cold finger of
a He continuous-flow cryostat.
Preparation of the Graphene
Reflector
A water-based
ink is prepared by ultrasonicating (Fisherbrand FB15069, Max power
800W) graphite flakes (Sigma-Aldrich) for 9 h in deionized water with
sodium deoxycholate (SDC, 9 mg mL–1). This is then
vacuum filtered using 100 nm pore-size nitrocellulose filters. This
blocks the flakes, while water passes through, leading to a film on
the surface of the filter. This is then placed on a 420-μm-thick
intrinsic high-resistivity Si/SiO2 double polished wafer
(acting as a back reflection mirror) and annealed at ∼80 °C
for 2 h, to improve adhesion, followed by dissolution of the filter
in acetone overnight.
Simulation of the Total GDD of the G sample
Numerical GDD simulations (Figure S2(a),(b)) are performed using a finite
element method (Comsol Multiphysics).
The simulated structure includes the end of the QCL waveguide and
a 65 nm thick GSA on a 420 μm thick SiO2/Si mirror,
separated by 15 μm from the laser back facet. This structure
is then surrounded at a distance of a few λ by vacuum and absorbing
boundary conditions. As the SiO2 layer is very thick (∼300
μm) compared to the separation between the GSA and the QCL facet,
the amount of radiation that could be reflected back to the QCL from
the SiO2/Si boundary is negligible. Thus, absorbing boundary
conditions are set ∼100 μm inside the SiO2, as well as at all the other external boundaries of the simulation
domain. The imaginary part of the refractive index of graphene is
computed from the experimental values of the absorption coefficients
reported in ref (30), while the real part is numerically computed considering a graphene
layer having a total scattering time τ = 0.1 ps and a chemical
potential μF = 250 meV. The variation of the imaginary
part under illumination from the QCL is computed according to the
expected reduction of the saturable absorption coefficient. The variation
of the real part is then computed applying the Kramers-Krönig
equations.THz radiation is injected into the QCL waveguide
(from the end opposite to the GTI) and then reflected back into the
QCL waveguide by the GTI. This allows us to obtain the amplitude and
phase of the S11 scattering parameter.[22,23] The dispersion provided by the structure is computed from the second
derivative of the phase. The final GDD profile takes into account
the contributions from the semiconductor material and gain of the
QCL,[23] and that of the GTI. The frequency
dependent refractive index of the material is computed using a Drude-Lorentz
model, adding its deviation due to the QCL’s gain, obtained
from the Kramers–Kronig equations. The waveguide dispersion
contribution, negligible with respect to the other terms, is neglected
All-Electrical Injection Locking of a Narrow Beatnote to an
RF Oscillator
The modulation signal is supplied by an external
stabilized RF synthesizer (Rohde & Schwarz SMA100B) through a
Bias-Tee (Tektronix PSPL5544). The beatnote signal is then extracted
from the bias line using the same bias-tee, and recorded with an RF
spectrum analyzer (Rohde & Schwarz FSW). For this, a high-speed
sub-miniature push-on (SMP) connector with an integrated coplanar
transmission line waveguide is used, allowing high-frequency electrical
signals to pass for fast electrical modulation, suppression of losses,
and deformation at the wire bonding points. The electrical connections
between one end of the QCL ridge and the coplanar probe are realized
using short and thin (20 μm) Au bonding wires.
Authors: Andrea C Ferrari; Francesco Bonaccorso; Vladimir Fal'ko; Konstantin S Novoselov; Stephan Roche; Peter Bøggild; Stefano Borini; Frank H L Koppens; Vincenzo Palermo; Nicola Pugno; José A Garrido; Roman Sordan; Alberto Bianco; Laura Ballerini; Maurizio Prato; Elefterios Lidorikis; Jani Kivioja; Claudio Marinelli; Tapani Ryhänen; Alberto Morpurgo; Jonathan N Coleman; Valeria Nicolosi; Luigi Colombo; Albert Fert; Mar Garcia-Hernandez; Adrian Bachtold; Grégory F Schneider; Francisco Guinea; Cees Dekker; Matteo Barbone; Zhipei Sun; Costas Galiotis; Alexander N Grigorenko; Gerasimos Konstantatos; Andras Kis; Mikhail Katsnelson; Lieven Vandersypen; Annick Loiseau; Vittorio Morandi; Daniel Neumaier; Emanuele Treossi; Vittorio Pellegrini; Marco Polini; Alessandro Tredicucci; Gareth M Williams; Byung Hee Hong; Jong-Hyun Ahn; Jong Min Kim; Herbert Zirath; Bart J van Wees; Herre van der Zant; Luigi Occhipinti; Andrea Di Matteo; Ian A Kinloch; Thomas Seyller; Etienne Quesnel; Xinliang Feng; Ken Teo; Nalin Rupesinghe; Pertti Hakonen; Simon R T Neil; Quentin Tannock; Tomas Löfwander; Jari Kinaret Journal: Nanoscale Date: 2015-03-21 Impact factor: 7.790
Authors: L Consolino; A Taschin; P Bartolini; S Bartalini; P Cancio; A Tredicucci; H E Beere; D A Ritchie; R Torre; M S Vitiello; P De Natale Journal: Nat Commun Date: 2012 Impact factor: 14.919
Authors: C A Zaugg; Z Sun; V J Wittwer; D Popa; S Milana; T S Kulmala; R S Sundaram; M Mangold; O D Sieber; M Golling; Y Lee; J H Ahn; A C Ferrari; U Keller Journal: Opt Express Date: 2013-12-16 Impact factor: 3.894