The performance of transistors designed specifically for high-frequency applications is critically reliant upon the semi-insulating electrical properties of the substrate. The suspected formation of a conductive path for radio frequency (RF) signals in the highly resistive (HR) silicon substrate itself has been long held responsible for the suboptimal efficiency of as-grown GaN high electron mobility transistors (HEMTs) at higher operating frequencies. Here, we reveal that not one but two discrete channels distinguishable by their carrier type, spatial extent, and origin within the metal-organic vapor phase epitaxy (MOVPE) growth process participate in such parasitic substrate conduction. An n-type layer that forms first is uniformly distributed in the substrate, and it has a purely thermal origin. Alongside this, a p-type layer is localized on the substrate side of the AlN/Si interface and is induced by diffusion of group-III element of the metal-organic precursor. Fortunately, maintaining the sheet resistance of this p-type layer to high values (∼2000 Ω/□) seems feasible with particular durations of either organometallic precursor or ammonia gas predose of the Si surface, i.e., the intentional introduction of one chemical precursor just before nucleation. It is proposed that the mechanism behind the control actually relies on the formation of disordered AlSiN between the crystalline AlN nucleation layer and the crystalline silicon substrate.
The performance of transistors designed specifically for high-frequency applications is critically reliant upon the semi-insulating electrical properties of the substrate. The suspected formation of a conductive path for radio frequency (RF) signals in the highly resistive (HR) silicon substrate itself has been long held responsible for the suboptimal efficiency of as-grown GaN high electron mobility transistors (HEMTs) at higher operating frequencies. Here, we reveal that not one but two discrete channels distinguishable by their carrier type, spatial extent, and origin within the metal-organic vapor phase epitaxy (MOVPE) growth process participate in such parasitic substrate conduction. An n-type layer that forms first is uniformly distributed in the substrate, and it has a purely thermal origin. Alongside this, a p-type layer is localized on the substrate side of the AlN/Si interface and is induced by diffusion of group-III element of the metal-organic precursor. Fortunately, maintaining the sheet resistance of this p-type layer to high values (∼2000 Ω/□) seems feasible with particular durations of either organometallic precursor or ammoniagas predose of the Si surface, i.e., the intentional introduction of one chemical precursor just before nucleation. It is proposed that the mechanism behind the control actually relies on the formation of disordered AlSiN between the crystalline AlN nucleation layer and the crystalline silicon substrate.
Access
to a plethora of physicn class="Chemical">al properties within the same semiconductor
family and simultaneous opportunity to design application-specific
heterostructures has generated tremendous interest in III-nitride
(Al, Ga, and In being the group-III elements)-based electronics in
the past two decades. Owing to the relentless device engineering[1−5] and the vital combination of wide band gap, high electron saturation
velocity, and ultralow channel resistance, AlGaN/GaN and InAlN/GaN
high electron mobility transistors (HEMTs) are now highly promising
candidates for microwave signal amplification. Unfortunately, the
lack of scalable and cost-effective III-nitride substrates has constrained
the realization of such functional layers to non-native platforms
such as SiC, sapphire, or silicon. Unparalleled large-area availability,
low-cost, and fabrication maturity make silicon the most commercially
attractive among the three. However, along with lattice mismatch,
epitaxy of III-nitrides on silicon brings the additional challenges
of melt-back etching[6,7] and stress management.[8,9] This has resulted in AlN nucleation[10,11] layers and
graded AlGaN buffers[12,13] becoming integral components
of III-nitride heterostructures grown on silicon. At times, the adverse
electrical implications of these additional layers have proven to
be a reason for concern, necessitating further scrutiny. In this context,
though the ill-effects of the AlGaN buffers in the form of leakage[14,15] and trapping[16,17] are now relatively well understood
and controlled, the suspected association of the AlN nucleation layer
with the formation of a conductive channel at the AlN/Si interface
is still under debate. Crucially, apart from thermal conductivity,
the power loss due to this channel has been alleged to be the remaining
bottleneck[18,19] for the high-frequency performance
(i.e., maximum power gain frequency and power output) of record-breaking
GaN-on-SiHEMTs[20,21] still lagging behind the devices
grown on SiC.[22,23]
With several mutun class="Chemical">ally exclusive
theories being discussed in the
scientific community, both the origin and the identity of this unintentional
substrate conductivity in metal-organic vapor phase epitaxy (MOVPE)-grown
heterostructures have always been controversial. For instance, an
inversion layer of electrons[24,25] arising from an abrupt
AlN/Si interface and oxy-nitride acceptor traps[26] due to a nonidealAlN/Si interface have both been independently
proposed to explain the presence of mobile carriers. Separately, group-III
elemental diffusion into the silicon substrate (and acting as acceptors)
has been attributed as the causal mechanism by several authors[27−33] alongside suggestions of diffusion partly arising from residual
species in the reactor.[27,29,32] Arguments negating the role of the substrate also exist, with the
AlN nucleation layer itself held accountable for being conductive.[34] Irrespective of the origin, the presence of
a capacitively coupled buried channel greatly undermines the potential
of GaN HEMTs by inducing power loss not only for the transistors but
also for the passive components and the connecting transmission lines
of the integrated circuits (ICs); for example, investigations on structures
grown by molecular beam epitaxy (MBE) process have identified that
controlling the epi/substrate interface is essential to minimize parasitic
conduction and radio frequency (RF) loss.[35,36] Given the superior growth rates and wafer throughput but also the
different thermodynamics and reaction kinetics of the MOVPE technique,
understanding and controlling the physical origin of the parasitic
conduction path in MOVPE-grown structures have become important to
the demonstration and large-scale production of high-performance GaN-on-Si
RF electronics. Using this motivation, the present investigation aims
to establish an unambiguous correlation between the observed buried
conductivity and the prenucleation stages of the III-nitride-on-Si
epitaxy. To achieve this, we investigate the origins of conductivity
in AlN-on-Si layers, which represent the initiation of the standard
HEMT growth process. After MOVPE deposition, we have implemented eddy
current-based resistance evaluation, Hall-effect measurement, and
scanning capacitance microscopy (SCM) to extract the magnitude, spatial
distribution, and carrier type of the conductive channels. In parallel,
we have analyzed the surfaces and the interfaces through atomic force
microscopy (AFM), secondary ion mass spectroscopy (SIMS), and cross-sectional
scanning transmission electron microscopy (STEM) with electron energy
loss spectroscopy (EELS) to provide a unified insight into channel
formation.
Results and Discussion
Epitaxy
of Aluminum Nitride on Silicon
Similar to RF n class="Chemical">Si-complementary
metal–oxide–semiconductor
(CMOS) devices, for high-frequency GaN-on-Si applications, it is customary
to grow upon highly resistive (HR) silicon wafers so that the power
loss due to substrate conductivity is at par with semi-insulating
GaAs.[37] Accordingly, Czochralski (CZ)-type
HR-Si(111) substrates (specified resistivity ≥3 kΩ cm)
were chosen for the study. Note that float-zone (FZ) HR wafers were
intentionally avoided given their higher cost and propensity to plastic
deformation (such as slip) at MOVPE process temperatures.[38,39] Prior to growth, noncontact RF eddy current induction-based evaluation[40] confirmed that sheet resistances (RSH) of all of the eight wafers were higher than the limit
of the measurement system (∼10 kΩ/□). On six of
these, a nominally 250 nm thick AlN nucleation layer was grown by
MOVPE under conditions typical of our standard HEMT structures.[15,41,42] In detail, this AlN layer growth
is divided into four steps, which are successively performed in the
reactor. Step-I (oxide desorption): in situ removal of the native
oxide on silicon by high-temperature (1080 °C) annealing in a
H2 ambient to generate a step-terraced surface; step-II
(precursor predose): short injection of either NH3 or trimethylaluminum
(TMAl) at 990 °C; step-III (low-temperature nucleation): growth
of ≈50 nm AlN with simultaneous NH3 and TMAl flow
at 990 °C; and step-IV (high-temperature growth): growth of the
remaining AlN layer with simultaneous NH3 and TMAl flow
at 1090 °C.
For step-II, both NH3 and n class="Chemical">TMAl predoses
may be discovered in the literature.[29,43−47] In this study, while keeping all of the other steps identical, the
predose step was varied with four durations (15, 60, 120, and 240
s) of NH3 flux at 40 μmol/s and two durations (6
and 12 s) of TMAl flux at 0.2 μmol/s to realize six uncracked
AlN-on-Si epistructures. Also, complete HEMT stacks were grown on
comparable AlN nucleation layers in separate process runs, comprising
additional deposition of a linearly graded AlGaN buffer, GaN buffer,
GaN channel, AlGaN barrier, and GaN cap of the standard structure.
All of these crack-free and low-bowed (∼50 μm, convex)
heterostructures showed a characteristic two-dimensional (2D) electron
gas (2DEG) density of ∼8 × 1012 cm–2, which confirmed their technological relevance. Also, as summarized
in Table , a reference
wafer was kept pristine for comparison (RS-1), i.e., not subjected
to any of the steps, whereas for another wafer (RS-2), the growth
process was terminated directly after step-I, i.e., before injecting
any precursor into the reactor.
Table 1
Summary of the Eight
Wafers Investigated,
including the Temperature and Duration of the Procedural Steps
structure
H2 anneal
precursor predose
250 nm AlN growth
reference substrate (RS-1)
−
−
−
reference
substrate (RS-2)
1080 °C, 30 min
−
−
AlN-on-Si templates (NH3 predosed)
1080 °C, 30 min
990 °C, (15/60/120/240) s
990 °C, 11 min+ 1090 °C, 80 min
AlN-on-Si templates (TMAl predosed)
1080 °C, 30 min
990 °C, (6/12) s
990 °C, 11 min+ 1090 °C, 80 min
Electrical, Structural, and Chemical Analysis
After growth, the RSH of n class="Chemical">all of the
AlN-on-Si wafers were measured again by the eddy current-based method,
and the resulting values are plotted in Figure . The figure shows two data sets at each
predose of NH3 (main graph) or TMAl (inset) representing
the RSH values for the as-grown structures
and after removal, by grinding, of 200 μm of material from the
backside of the Si substrate. Among the wafers with full thickness,
the average RSH of RS-2 was reduced to
596 Ω/□ by just the processes in step-I of the growth
(up to and including the H2 anneal), a change of almost
2 orders of magnitude. With as-grown AlN, the RSH were even lower, but the exact value was predose-dependent;
for example, increasing the duration of NH3 predose resulted
in a systematic increase of RSH from 279
to 441 Ω/□, whereas increasing the TMAl duration caused
a small decrease from 427 to 409 Ω/□. Thinning of the
substrate was performed to remove any effects of group-III diffusion
into the backside of the Si wafer, which could result from residual
contamination of the susceptor (on which the substrate is placed),
and as the eddy current-based method measures the full thickness of
the sample, it would contribute to the measured conductance. As shown
in Figure , after
thinning, the RSH of thinned RS-2 was
1058 Ω/□, whereas RSH for
the thinned templates varied from 393 to 691 Ω/□ for
the NH3 predose and from 645 to 491 Ω/□ for
the TMAl predose, retaining the same qualitative dependence on predose,
although at higher values. The presence of conductivity in all of
the wafers even after backside grinding indicates the presence of
sources of carriers in addition to/distinct from backside contamination.
However, the fact that measurements of RS-1 after thinning yielded
a characteristic ≥10 kΩ/□ value (not shown) allows
any influence of the grinding process itself on conductivity to be
ruled out.
Figure 1
Dependence of AlN-on-Si average sheet resistance on the NH3 predose duration. The inset shows the dependence for the
TMAl predose durations. The two data at each predose represent the
values for as-grown structures (symbol: circle) and after 200 μm
backside grinding (symbol: square). For reference, the measured values
of the annealed substrate (RS-2) are also shown in the plots.
Dependence of AlN-on-n class="Chemical">Si average sheet resistance on the NH3 predose duration. The inset shows the dependence for the
TMAl predose durations. The two data at each predose represent the
values for as-grown structures (symbol: circle) and after 200 μm
backside grinding (symbol: square). For reference, the measured values
of the annealed substrate (RS-2) are also shown in the plots.
To understand
whether any
of the decrease in RSH of RS-2 was caused
by elementn class="Chemical">al diffusion into the front surface of the wafer during
the annealing step, which would then similarly affect the AlN-on-Si
templates, the near-surface region of the thinned RS-2 was scrutinized
by SIMS.
As shown in Figure , none of the group-III species used in the reactor
had any variation
suggestive of an in-diffusion process (the profiles at ≤50
nm from the surface are not “ren class="Chemical">al” features) and were
below the SIMS detection limit. This not only attests to the success
of the strictly followed reactor purge routines but also confirms
that the conductivity measured in RS-2 after annealing does not arise
from residual[27,29] Al or Ga. Importantly, as shown
in the inset, it was also confirmed that none of the probable contaminants
such as C, N, or H had diffused into the substrate either. It is worth
mentioning that the N depth profile with a sharp increase near the
surface was similar to that observed by Chandrasekar[26] et al., who linked such a variation with the conductivity
of AlN-on-Si through an alleged formation of a Si–O–N
complex. We argue that such rapid decays within ∼100 nm from
the sample surface (or interface) are more likely to be an artificial
feature for adventitious surface species (or resputtered matrix effect).
Among all of the inspected elements, only O had a depth-dependent
variation indicative of out-diffusion marked by an increase up to
3 μm depth, beyond which this interstitial species[48] is expected to level off at the bulk concentration
of mid-1017 cm–3 for Czochralski (CZ)-grown
silicon.
Figure 2
SIMS evaluated atomic concentration of different group-III species
in the silicon substrate that was annealed under H2 ambient
(RS-2). The corresponding profiles of other probable contaminants
are shown in the inset. Except oxygen, none of these exhibited any
meaningful variation within the probed depths and were at their respective
detection limit. In both the graphs, the origin of the x-axis denotes the top silicon surface.
SIMS evn class="Chemical">aluated atomic concentration of different group-III species
in the silicon substrate that was annealed under H2 ambient
(RS-2). The corresponding profiles of other probable contaminants
are shown in the inset. Except oxygen, none of these exhibited any
meaningful variation within the probed depths and were at their respective
detection limit. In both the graphs, the origin of the x-axis denotes the top silicon surface.
To clarify the carrier type and densities giving rise to the measured
conductivity, scribed samples from n class="Chemical">all wafers were then subjected
to Hall-effect measurements. While attempts were made to contact the
samples from both the AlNside and rear of the wafers, the measured I–V characteristics of these samples
indicated that only contacts on the backside of the silicon were ohmic.
The Hall coefficients (RH) were confirmed
to be negative for all of the specimens indicating that the dominant
carriers were electrons. The calculated areal densities averaged from
three to six samples of each wafer are listed in Table , and within the small test
population, no significant variation was observed, with average values
ranging from 4.2 × 1012 to 6.3 × 1012 cm–2, which is similar to the 5.2 × 1012 cm–2 observed for RS-2. Since these carriers
could be either evenly distributed through the thickness of the Si
or form a localized layer, additional depth-dependent Hall-effect
measurements were carried out in an attempt to identify any evidence
for the proposed inversion layer localized at the AlN/Si interface
that would host a similar sheet carrier density.[25] For these measurements, separate samples were scribed and
then polished from either the backside or the topside to reduce their
thickness. Note that thinning from the topside involved complete removal
of the AlN and its interface with silicon. As detailed in Table , the thinned samples
showed a decrease in areal carrier density that was clearly proportional
to the decrease in thickness. These experiments along with the similar
value for carrier density in RS-2 and all of the templates proved
that electrons causing this unintended conductivity were actually
distributed throughout the thickness of the bulk silicon with an approximate
volume concentration of mid-1013 cm–3. Notably, even after thinning, no specimens from RS-1 could be probed,
reconfirming that the modified substrate conductivity was indeed annealing
or growth process-induced.
Table 2
Hall-Effect Measurement
Results on
Samples from the Annealed Si Wafer and the AlN-on-Si Structures with
Different Predosesa
only H2 annealed (RS-2)
NH3/15 s
NH3/60 s
NH3/120 s
NH3/240 s
TMAl/6 s
TMAl/12 s
series-A: e– density (1012 cm–2)
5.2 ± 0.8
5.7 ± 0.3
4.4 ± 0.3
5.1 ± 0.5
4.2 ± 0.1
6.3 ± 0.5
5.6 ± 0.9
series-B: e– density (1012 cm–2)
4.9 (750/T)
2.9 (450/B)
2.8 (460/B)
2.4 (450/T)
Series-A: mean
and uncertainty values
for several samples from each wafer with an 800 μm substrate
thickness. Series-B: as-measured value for further thinned samples
from particular wafers. For series-B, the final sample thickness (in
μm) and the side from which the material was removed are mentioned
inside the brackets as T: AlN topside and B: silicon backside.
Series-A: mean
and uncertainty values
for severn class="Chemical">al samples from each wafer with an 800 μm substrate
thickness. Series-B: as-measured value for further thinned samples
from particular wafers. For series-B, the final sample thickness (in
μm) and the side from which the material was removed are mentioned
inside the brackets as T: AlN topside and B: silicon backside.
Nonetheless, the above-mentioned
electricn class="Chemical">al measurements do not
exclude the presence of an additional interfacial channel and in fact
the variation in RSH with predose duration
shown in Figure strengthens
this notion. To inspect the details of any conductivity arising adjacent
to the AlN/Si interface, cross-sectional scanning capacitance microscopy
(SCM) was carried out. This electrical variant of contact-mode atomic
force microscopy (AFM) utilizes the bias-dependent differential capacitance
of the tip-to-semiconductor junction and simultaneously acquires topography
and a local charge-carrier data map.[15,49,50] The measurements were carried out on cleaved cross
sections. First, the upper edge of the cross section above the AlN
layer was identified from an abrupt and characteristic increase of
the measured deflection error. Then, using the thickness of the AlN
as a guide, approximately 10 μm into the silicon substrate was
scanned for samples from all of the templates.
Figure shows the
representative topography and dC/dV phase (Δϕ = ϕ – ϕL, where
ϕL is the lock-in phase) map of a 1.5 μm ×
10 μm (width × depth) subsurface region from the structure
with a 15 s NH3 predose. In SCM, phases of the conducting
regions can be used to asn class="Chemical">sign the carrier type. The bimodal distribution
in the phase maps of Figure reveals that the phase responses for the two conducting regions
are 180° out of phase indicating opposite carrier polarity. Referencing
the buried conducting region (Δϕ ∼ −90°)
in the maps as the newly formed bulk n-type layer in silicon, the
channel (Δϕ ∼ +90°) present at the AlN/Si
interface is clearly p-type. This presence of both types of carriers
was observed in the cross-sectional scan of every AlN-on-Si structure.
Notably, on some samples, the buried layer did not appear at zero
DC bias but superimposing a DC bias during the scans revealed that
this layer was indeed present (see the Supporting Information). As for the p-type layer, though some variation
in the depth of this region was observed within samples, its presence
was clearly identifiable in all of the samples at zero DC bias irrespective
of the predose type and duration. Without a calibration staircase[49] within the AlN-on-Si structure, quantitative
calculations of hole concentrations are not possible from the SCM
data itself. Nonetheless, the presence of this additional layer explains
the cause of further decreased sheet resistance in the epistructures
compared to that of the annealed substrate.
Figure 3
Three-dimensional (3D)
topography and 2D dC/dV phase map
from a cross-sectional specimen of the 15 s
NH3 predosed AlN-on-Si structure. The approximate position
of the AlN/Si interface is indicated by a dashed line in the topography
image. The phase map validates that carriers of the two conducting
layers in silicon have opposite polarity (Δϕ ∼
+90° and −90°, represented as white and dark regions,
respectively) and they are separated by a zone lacking free carriers
(Δϕ ∼ 0°, gray region). From this phase response,
the carriers can be designated as shown in the color-coded carrier
map schematic. The near-surface carriers are identified as holes,
whereas the buried carriers are identified as electrons along with
a region lacking carriers between the two conducting layers. Note
that the roughness arising from cleavage planes and morphological
features of the sidewalls had minimal influence on the overall phase
data.
Three-dimensionn class="Chemical">al (3D)
topography and 2D dC/dV phase map
from a cross-sectional specimen of the 15 s
NH3 predosed AlN-on-Si structure. The approximate position
of the AlN/Si interface is indicated by a dashed line in the topography
image. The phase map validates that carriers of the two conducting
layers in silicon have opposite polarity (Δϕ ∼
+90° and −90°, represented as white and dark regions,
respectively) and they are separated by a zone lacking free carriers
(Δϕ ∼ 0°, gray region). From this phase response,
the carriers can be designated as shown in the color-coded carrier
map schematic. The near-surface carriers are identified as holes,
whereas the buried carriers are identified as electrons along with
a region lacking carriers between the two conducting layers. Note
that the roughness arising from cleavage planes and morphological
features of the sidewalls had minimal influence on the overall phase
data.
SCM phase data yields no fixed
value when scanning insulating regions,
or regions of extremely low carrier concentration, due to the lack
of carriers to modulate. Such insulating regions appear as noise in
typicn class="Chemical">al SCM images. Between the p-type and the n-type regions, there
is such a noisy band in the phase maps with ϕ ∼ ϕL. This likely arises from an equilibrium depletion region
between the conducting layers. Previously, Matsumoto[29] et al. observed in scanning spreading resistance microscopy
(SSRM) a gradual decrease followed by an abrupt drop of carrier concentration
below the AlN/Si interface in GaN/AlN/Si structures. The authors had
credited the latter effect to passivation of carriers by diffused
H2. The lack of carrier-type information from the SSRM
data and the limited scan size (∼3 μm) of their study
precludes a direct comparison with our data. However, the results
are consistent with the presence of a hole channel followed by a depletion
region, similar to that observed here.
Very recently, the presence
of a p-type layer followed by a depletion
region that is formed with the FZ-grown n-type substrate has been
evidenced by Bah[32] et n class="Chemical">al. through coupled
SCM and SSRM experiments. For AlN grown with a fixed NH3 predose, those authors had observed a proportional relationship
between the AlN growth temperature and the width of the p-type layer.
Though such a systematic variation of the p-type layer width could
not be established for the present structures, its existence localized
at the AlN/Si interface indeed explains the source of decreased sheet
resistance in the epistructures compared to that of the annealed silicon
substrate, and our data shows that the conductivity of this channel
can be varied with the predose type and duration. In view of the Hall-effect
results, assuming the sheet resistance of the bulk n-type regions
to be invariant for all of the structures and equal in magnitude with
RS-2, the specific RSH of the p-type layer
were extracted for each template. For the samples with an NH3 predose, the plotted values in Figure first show a rapid increase from 602 to
1644 Ω/□ with increase in the duration from 15 to 60
s but become approximately constant for predose times between 120
and 240 s at around 2000 Ω/□. In contrast, a fast decrease
from 1824 to 869 Ω/□ can be seen for increasing TMAl
predose from 6 to 12 s. As RSH = ρchannel/t, where ρ and t denote the channel resistivity and thickness, considering t of the SCM-resolved p-type layer to be ∼3 μm
and approximating a uniform distribution, these values reveal an associated
resistivity of ∼0.2–0.6 Ω cm, suggesting[51] 1016–1017 cm–3 acceptors on average for the whole layers. Notably,
such magnitudes of unintentional doping agree well with both the estimated
volume concentration of holes[32] in the
p-type layer and the ranges of the reported[26,27,29] SIMS depth profiles for group-III species.
Also, in conjunction with the Hall effect-measured n-type carrier
concentrations (i.e., mid-1013 cm–3),
these values of p-type carriers should result in a p–n junction
depletion region of ∼4 μm, quite consistent with those
observed in SCM.
Figure 4
Calculated average sheet resistances of the p-type layer
for increasing
durations of the NH3 predose. These show an initial increase
followed by saturation. Corresponding values for the TMAl predoses
in the inset reveal a fast decrease instead. All of the calculations
assume that the n-type and p-type layers independently conduct in
parallel.
Calculated average sheet ren class="Chemical">sistances of the p-type layer
for increasing
durations of the NH3 predose. These show an initial increase
followed by saturation. Corresponding values for the TMAl predoses
in the inset reveal a fast decrease instead. All of the calculations
assume that the n-type and p-type layers independently conduct in
parallel.
Importantly, it becomes
obvious that for the inspected flow rates, NH3 provides
a larger predon class="Gene">sing window within which RSH values remain high, which could be beneficial for run-to-run reproducibility
of the electrical performance of the as-grown HEMTs. On the other
hand, shorter optimization window seems inherent to the TMAl predose,
as for similar reaction kinetics (∼0.3 μmol/s at 980
°C), changes of TMAl flow duration from just 6 to 24 s have been
reported[29] to increase the diffused aluminum
density from ∼1012 to ∼1015 cm–2.
As an indicative measure of the adverse influence
of these unintentional
conductivities on the high-frequency performance, transmisn class="Chemical">sion losses
were evaluated from the scattering parameters of coplanar waveguides
(CPWs) fabricated on the AlN surfaces (plotted in Figure ). As shown, for all of the
frequencies, the losses were similarly low for the structures with
higher sheet-resistance values (60, 120, and 240 s NH3 predoses
and 6 s TMAl predose) but were considerably higher for both 12 s TMAl
and 15 s NH3 predoses. In fact, at 40 GHz, more than half
of the signal power (−3 dB) was attenuated for the latter.
Figure 5
Measured
small-signal propagation loss as a function of frequency
for ground-signal-ground CPW lines fabricated on the AlN grown with
either TMAl or NH3 predose. The data confirms a correlation
between the high-frequency loss and previously measured epistructure
sheet conductance. A 1 × 1 mm2 optical micrograph
of the fabricated transmission lines and on-chip calibration structure
are shown in the inset.
Measured
small-signal propagation loss as a function of frequency
for ground-signal-ground CPW lines fabricated on the AlN grown with
either TMAl or NH3 predose. The data confirms a correlation
between the high-frequency loss and previously measured epistructure
sheet conductance. A 1 × 1 mm2 optical micrograph
of the fabricated transmission lines and on-chip calibration structure
are shown in the inset.Radiation losses being
negligible in the probed frequency range,[34] attenuations during signn class="Chemical">al propagation on such
metal-dielectric waveguides primarily originate from the nonideality
of the materials in the form of dielectric loss and conductor loss.
The latter is known to be the dominant factor at <1 GHz and is
controlled by surface resistivity and line inductivity, which should
be similar for all of the identically deposited metallic lines. Effectively,
this indicates that the sample-to-sample variation in measured loss
is due to the varying contribution of dielectric loss. It is also
known that for a dielectric (AlN–Si composite in this case),
the losses[34,52] are dependent on the dielectric
conductivity in the form of effective loss tangent (tan δd_eff) aswhere the first term represents the dielectric
damping, and the second represents the dielectric conduction with
σ, ε, and f being the conductivity, permittivity,
and frequency, respectively. Thus, as the dielectric loss at any particular
frequency is directly dependent on the conductivity, the observed
variation in signal attenuation among the present structures further
accentuates the role of predose in minimizing the losses for GaN-on-SiHEMTs. Also, as listed in Table , the losses increase with increase in frequency. Based
on the spatial extents of the conductive layers, it is plausible that
at lower frequencies the effect of the p-type layer is dominant, and
at higher frequencies, capacitive coupling superimposes the effect
of the bulk electrons. It must be emphasized that dielectric losses
on thick epilayers are proportionate to the losses on corresponding
AlN-on-Si templates[31] as high-frequency
signals penetrate deep into the substrate. Thus, the observed predose
dependence is expected to persist for fabricated devices that would
be several microns away from the AlN/Si interface.
Table 3
Comparison of Propagation Losses (in
dB/mm) at Specific Frequencies for 100 μm Long CPW Transmission
Lines Fabricated on AlN-on-Si Structures Grown with Different Predoses
NH3/15 s
NH3/60 s
NH3/120 s
NH3/240 s
TMAl/6 s
TMAl/12 s
loss at 5 GHz
22.6
13.1
12.7
14.2
13.8
16.1
loss at 10 GHz
24.9
14.1
14.1
15.7
15.1
18.0
loss at 50 GHz
30.1
17.5
17.9
19.0
18.7
22.4
To elucidate the mechanisms
behind the effects of the prenucleation
growth stages on the interfacial carrier formation, we have further
investin class="Chemical">gated the microstructures of the various samples. First, the
as-grown AlN surfaces were scanned by AFM in tapping mode. Representative
5 × 5 μm2 images for different NH3 predoses are shown in Figure a–d and indicate the influence of the 15–240
s predose step on the finalAlN surface. The predominantly flat surfaces
were found to contain pits whose depths, widths, and density were
dependent upon the predose duration. Further magnified scans revealed
that the pit openings were aligned with crystallographic directions
(see the Supporting Information). As AlN
is unlikely to be etched by H2 at the growth temperatures,
these pits are suggestive of aligned crystallites in the process of
coalescing with one another. As a measure of this coalescence process,
two parameters, namely, the fractional surface area of pits and their
maximum depths, were evaluated for each wafer. Understandably, a more
coalesced layer should possess a reduced value for both entities.
The corresponding trends in Figure e demonstrate that as the predose duration increased
from 15 to 240 s, the morphology changed from complete merger of the
crystallites to ∼7% noncoalesced area. In parallel, the maximum
probed pit depth also increased by an order of magnitude though as
the size of the individual pits gets smaller, depths are likely to
be underestimated due to the AFM tips’ inability to access
the bottom of high-aspect-ratio holes. The topographies for the TMAl
predoses largely resembled that of the 15 s NH3 predose
(see the Supporting Information). Notably,
regardless of the predose type/duration before AlN nucleation, the
final surface topography after growth of subsequent layers of the
complete HEMT structure was always identical and completely coalesced
(see the Supporting Information). However,
as the CPW lines were directly fabricated on top of the AlN surfaces,
the presence of larger voids for longer NH3 predoses may
have caused additional scattering of the propagating RF signal. This
may explain the slightly higher losses for 240 s compared to those
for 60 and 120 s NH3 predosed structures at all frequencies,
as shown in Figure .
Figure 6
AFM surface topography of 250 nm AlN epilayers grown with NH3 predose durations of (a) 15 s, (b) 60 s, (c) 120 s, and (d)
240 s indicates a continuous decrease in coalescence with increase
in duration. In all of the scans, the height scales represent 10 nm.
The normalized noncoalesced area and the maximum probed depth for
each predose are quantified in (e) averaged from three 5 × 5
μm2 scans on each wafer.
AFM surface topography of 250 nm AlN epilayers grown with n class="Chemical">NH3 predose durations of (a) 15 s, (b) 60 s, (c) 120 s, and (d)
240 s indicates a continuous decrease in coalescence with increase
in duration. In all of the scans, the height scales represent 10 nm.
The normalized noncoalesced area and the maximum probed depth for
each predose are quantified in (e) averaged from three 5 × 5
μm2 scans on each wafer.
Further investigation of the microstructure used cross-sectionn class="Chemical">al
STEM-EELS investigations of the AlN/Si interface. For this experiment,
lamellae from two different HEMT structures having 60 and 240 s NH3 predosed AlN were prepared for cross-sectional viewing in
STEM mode. As depicted in the low-magnification, high-angle annular
dark-field (HAADF) image of the 60 s predosed structure (Figure a), the presence
of a dark interlayer between the AlN and the Si was prominent in both
the specimens. The absence of channeling in the region suggests disorder
and/or intermixing. To chemically identify this interlayer, EELS spectra
were acquired from the interfaces, and the high-loss energy range
between 70 and 130 eV was scrutinized to probe the different bonding
states of Si and Al atoms. It was seen that the Si–L23 edge near the interface had an energy shift compared to Si-bulk,
owing to charge redistribution[46] from Si
bonded to Si and Si bonded to nitrogen in SiN. In addition, the spectra revealed that near the interface (see
the Supporting Information), Al–L23 edge had shifted from the expected position of Al in AlN
or Al to an intermediate bonding state, which does not correspond
to a known reference compound, which we have termed as Al*. The 2D
EELS intensity map around the AlN/Si interface of the 60 s NH3 predosed sample is shown in Figure b. In Figure c–f, separate maps of the different signals
at this interface are given, which show the following features:
Figure 7
(a) HAADF-STEM micrograph of the 60 s NH3 predosed
structure
showing the presence of a disordered region at the AlN/Si interface.
(b) EELS integrated intensity map from a representative (21 ×
81) pixel image of the same interface. The individual chemical profiles
were extracted from this EELS signal, and the respective extents are
shown in (c)–(f) as intensity maps. The horizontal scale bars
in (b)–(f) represent 3 nm. From such multipixel images, averaged
intensity profiles of different Si and Al states across the interface
are plotted in (g) and (h) for 60 and 240 s NH3 predoses,
respectively (all of the profiles are normalized to their individual
maximum intensity value, and error bars represent standard errors
of the measurement). In both the plots, the zero of the x-axis corresponds to the peak of the fitted Si(SiN) profile, and the calculated full width at half-maxima
(FWHMs) of the same are marked. Note the heterogeneity of the Si(SiN)/Al(AlN) interface.
Sin class="Chemical">signal corresponding
to elementalSi is seen to the left of Figure c, specifying the position of the silicon substrate.
Aln class="Chemical">signal corresponding
to AlN is seen
to the right of Figure d, specifying the position of the AlN layer.
Sin class="Chemical">signal corresponding to SiN is seen as a band in the center of Figure e, positioned between
the silicon substrate and the AlN layer.
Al* n class="Chemical">signal is seen as a band in the
center of Figure f,
also positioned between the silicon substrate and the AlN layer.
(a) HAADF-STEM micrograph of the 60 s NH3 predosed
structure
showing the presence of a disordered region at the n class="Chemical">AlN/Si interface.
(b) EELS integrated intensity map from a representative (21 ×
81) pixel image of the same interface. The individual chemical profiles
were extracted from this EELS signal, and the respective extents are
shown in (c)–(f) as intensity maps. The horizontal scale bars
in (b)–(f) represent 3 nm. From such multipixel images, averaged
intensity profiles of different Si and Al states across the interface
are plotted in (g) and (h) for 60 and 240 s NH3 predoses,
respectively (all of the profiles are normalized to their individual
maximum intensity value, and error bars represent standard errors
of the measurement). In both the plots, the zero of the x-axis corresponds to the peak of the fitted Si(SiN) profile, and the calculated full width at half-maxima
(FWHMs) of the same are marked. Note the heterogeneity of the Si(SiN)/Al(AlN) interface.
To quantify the spatial extent of these different bonding states,
the extracted spectra for each species were then averaged as a function
of width n class="Chemical">along the interface. The resulting chemical profiles, integrated
across the interface, are plotted for 60 and 240 s NH3 predoses
in Figure g,h, respectively.
From the extracted intensities, the fitted widths for the Si(SiN) profile reveal FWHMs of 3.7 ± 0.2 and
5.3 ± 0.2 nm for 60 and 240 s of NH3 predose, respectively.
In addition, comparable width and significant spatial overlap of the
Al* profile in both the instances suggest that instead of binary SiN that has been suggested till date,[30,43,46,53,54] an intermixed AlSiNalloy exists at the
AlN/Si interface. The thicknesses further confirm that for NH3 predoses, a higher duration leads to a thicker layer between
the Si substrate and the low-temperature AlN nucleation layer. A detailed
spectroscopic analysis on this interlayer will be published separately.
Origins of the Carriers and the Role of
the Predose
Given the electrical and structurn class="Chemical">al characteristics
of the wafers, it is evident that the overall conductivity comprises
distinct origins. To begin with, the drastic fall in sheet resistance
of the annealed substrate along with the uniform concentration of
electrons throughout the bulk indicates the formation of thermally
generated donors during the heating of the Si wafer. Hence, the high
resistivity of the substrate is not impervious to high temperatures
in a H2 ambient, and even the 30 min long oxide desorption
step at 1080 °C is sufficient to significantly reduce the initial
resistivity of the HR-Si. The implication of the thermal cycling on
the conductivity of Si wafers has not been widely recognized in the
III-nitride growth literature despite the reduction of resistivity
and reversal in majority carrier type as a result of thermal annealing
being understood since the earliest Si microwave ICs.[55] The source of this bulk conductivity is likely associated
with the generation of one or multiple thermally induced donors.[56−58] Oxygen precipitates are plausible candidates considering the high
levels of intrinsic oxygen present in CZ-grown Si. Passivation of
residual substrate impurities by hydrogen[38] during the high-temperature annealing step cannot be ruled out either.
Further work understanding the role of the thermal profile of the
Si during the growth of III-nitride heterostructures may allow control
or at least reduction of their concentration. This would not only
decrease the overall conductance of the n-type layer but also increase
the p–n junction depletion width, which, owing to the difference
in p- and n-carrier concentrations, primarily penetrates into the
n-region. Effectively, this would reduce the capacitive coupling of
devices to these electrons and could complement processing-based approaches
of thinning or local substrate removal[28,59] to provide
a viable option to circumvent this bottleneck. It is worth mentioning
that additional diffusion of susceptor contaminants through the backside
of the silicon at high temperatures may have contributed to the measured
sheet resistance of the wafers with full thickness. This is derived
from the fact that only for the generated bulk electrons, the RSH of the annealed substrate, i.e., RS-2 with
1000 μm thickness, should have been approximately 840 Ω/□
instead of the much lower 596 Ω/□ that
was measured. While this backside conductivity far away from the device
plane is not considered to be important for the operation of GaN-on-SiHEMTs and can be removed by simple backside grinding, it clearly contributes
to the eddy current measurement and must be considered for wafer level
measurements.
In view of other possible sources, the interfacin class="Chemical">al
AlSiN is a disordered alloy and is expected to have low mobility and,
hence, is unlikely to contribute to the high-frequency conductance.
However, in comparison to the distributed n-type layer evidenced above,
the p-type layer at the AlN/Si interface has significantly higher
conductivity and would also have closer capacitive coupling with the
2DEG channel in a HEMT. It is emphasized that though all of the AlN
layers were thicker than the proposed limiting thickness[24] for inversion electrons, any evidence of interfacial
electrons was absent. As for the holes, the agreement of the SCM-observed
distribution of the p-type region with the reported SIMS depth profiles
of Al reported in the literature confirms that the holes are indeed
of extrinsic origin arising from group-III elemental in-diffusion.
The SIMS depth profile of RS-2 further proves that this diffusion
does not occur prior to the injection of organometallics into the
reactor. Hence, for the NH3 predosed AlN-on-Si templates,
diffusion must have occurred during the nucleation period that ends
once the silicon is covered with AlN and/or during the rest of the
bulk AlN growth. It is noted that SiN has been proposed to act as a diffusion barrier,[27] and it has also been suggested[9,43] that
even with an amorphous SiN, through the
interface Si–SiN–AlN crystalline, relationship is maintained
by intermittent local zones where the SiN is discontinuous. In this context, higher NH3 predoses
are expected to result in thicker interlayers (as observed) and provide
more coverage of the exposed silicon, both plausibly prohibiting direct
diffusion of Al during the nucleation phase. If significant diffusion
during the bulk growth period takes place instead, defects such as
grain boundaries and dislocations are expected to facilitate the process.
Increasing the NH3 predose duration has been reported[43−45] to yield lower dislocation density in GaN buffer, and a commensurate
density reduction in the AlN nucleation layer[45] itself has been suggested as the underlying cause. Based on the
observed delay in coalescence with increase in the predose duration,
we anticipate that thicker SiN functions
as more efficient local masks[60,61] to reduce the dislocation
densities. Theoretically[62] and experimentally,[63,64] dislocations have been proposed to act as diffusion pathways in
III-nitrides. Though the diffusivity of Al through dislocations in
AlN and its dependence on the core structure is yet to be reported,
as longer NH3 predoses likely reduce the dislocation density,
those may have reduced dislocation-mediated diffusion during the subsequent
bulk growth period as well. On the other hand, increasing the NH3 predose duration definitely increases the density of pits,
but the anticorrelation between the pitted area and RSH proves that pit defects are not major contributors
to the diffusion process.
In contrast to the NH3 predose,
growths using TMAl predose
provide an opportunity for direct “Al” diffusion during
the predose period itself. Thus, for fixed flow rates, increasing
the TMAl predose duration could enhance the density of the group-III
species in the substrate by enabling diffusion before nucleation.
A progressive increase of the amount of Al in the substrate with longer[29] TMAl predoses supports such a mechanism and
may explain the relationship between TMAl predose duration and extracted RSH for the present structures. However, for
the short TMAl predose (6 s), the high sheet resistance of the p-type
layer confirms that the diffusion during the nucleation and the bulk
growth can indeed be restricted to the amounts comparable to the optimized
NH3 predoses. Notably, TMAl predosed AlN have also been
consistently shown[30,46,53,54] to include a prominent SiN layer forming either from the background “N”
sources or during the first growth phase when both “Al”
and “N” are simultaneously present on exposed silicon.
For TMAl predosed structures, evaluation of the interface, morphology,
and sheet-resistance/diffused Al density at different stages of growth
can further reveal the role of SiN in
post-predose diffusions. Understanding of the diffusion pathways that
are active during the latter stages of AlN-on-Si growth is important
as they explain the observations[24,31] of higher
RF losses suffered by thicker AlN layers (i.e., longer growth/diffusion
times) grown at the same temperature (i.e., same activation energy),
independently of the “inversion channel” theory.
Conclusions
Systematic electrical and materin class="Chemical">al characterizations
have established
that the origin of parasitic substrate conduction in MOVPE-grown GaNHEMT heterostructures on HR silicon stems from separate growth-related
sources. A substantial reduction in the resistivity of the Czochralski-type
silicon substrate just after the high-temperature native oxide desorption
step was revealed, and bulk electrons originating from thermally generated
donors were attributed as the source of this conduction. In addition,
the debated conductive layer at the AlN/Si interface was confirmed
to be p-type and most likely originating from group-III acceptors,
which had diffused several microns into the substrate. It was observed
that for particular durations, initiating the growth with either the
hydride (i.e., NH3) or the organometallic precursor (i.e.,
TMAl) predose resulted in similar high sheet resistance (∼2000
Ω/□) of this p-type layer. It is possible that elemental
diffusion occurs before, during, or postnucleation of the AlN layer
and the efficacy of different predoses is associated with inhibiting
the diffusion at different stages of the growth. Also, though the
high-frequency signal attenuation was seen to be related to the epistructure
sheet resistances, simulations of electromagnetic energy propagation
through such lossy dielectrics are needed to distinguish the contribution
of the distributed n-type and the localized p-type layer. To date,
the high-temperature performance of GaNHEMT on HR-Si has been simulated[65] based upon the assumption that the intrinsic
resistivity of the substrate stays intact even after growth. Based
on present findings, it is anticipated that such guidelines will necessitate
a re-evaluation. Also, FZ Si intrinsically has lower oxygen levels
and may provide better immunity against the thermal generation of
bulk donors. However, they would not prevent the unintentional group-III
doping close to the AlN/Si interface, which can only be controlled
by the predose. In parallel, device architectures,[66,67] which are less prone to substrate conductivity, may see increasing
adaptations. Notably, additional conductivity was also suspected at
the back face of the silicon substrates, although this is sufficiently
separated from the active device layers that it will not have an impact
on device performance.
Materials
and Methods
Metal-Organic Vapor Phase Epitaxy (MOVPE)
Growth
All of the epilayers investin class="Chemical">gated in this study were
grown in an Aixtron 1 × 6 MOVPE reactor with a close-coupled
showerhead (CCS) geometry. The growth temperatures and temperature
uniformities were controlled by in situ calibrated pyrometers of an
EpiTT module (emissivity-corrected) and an Argus photodiode array
module, respectively. During growth, the thicknesses and surface morphologies
were monitored in real time by interferometry at three different wavelengths
(405, 633, and 950 nm). Electronic-grade (7 N) trimethylaluminum (TMAl,
Dow Chemicals), trimethylgallium (TMGa, SAFC), and ammonia (NH3, BOC) were used as the precursor for Al, Ga, and N, respectively.
Pd-cell-purified hydrogen (H2, Air Products) with a dew
point of −120 °C (moisture level <50 ppb) was used
as the carrier gas. The 1 mm thick 6 in. Czochralskisilicon wafers
(supplied by Shin-Etsu Handotai) used for the growths had a specified
resistivity of 3–10 kΩ cm. Each growth experiment was
followed by manual scraping and brushing of the showerhead to remove
deposits from previous depositions and a high-temperature bake. The
reactor was continuously purged with nitrogen between runs/bakes.
The RSH of intact
6 in. wafers were measured in an LEI 1510 instrument that induces
eddy currents in the semiconductor by oscillating magnetic fields
that are coupled through an RF tank circuit. The power absorbed in
the materin class="Chemical">al is converted to conductance with reference to calibrated
standards. The probed area for each measurement was ∼1.5 cm2, and 51 separate positions were measured for each wafer.
Secondary Ion Mass Spectroscopy (SIMS)
SIMS depth profile in the n class="Chemical">silicon was measured by EAG Laboratories,
either with Cs+ primary beam (to detect H, C, N, and O
as negative ions) or with O2+ primary beam (to
detect B, Al, and Ga as positive ions) having beam energies 1–30
keV. The top surface of a scribed specimen from the oxide-desorbed
silicon substrate (RS-2) was subjected to the analysis.
Hall-Effect Measurement
First 1
× 1 cm2 square specimens were scribed from each wafer,
and indium contacts were soldered (300 °C for 60 s) at the four
corners to ren class="Chemical">alize the van der Pauw (vdP) geometry. For the 800 μm
thick AlN-on-Si specimens, only the contacts on the backside silicon
were found to be ohmic. These contacts were used for four-probe Hall-effect
measurements in an Ecopia HMS 5500 system with 560 mT magnets. After
complete removal of AlN by polishing, ohmic behavior could be realized
with topside contacts as well. For the untreated silicon wafer (RS-1), I–V curves could not be acquired
due to the excessively high potential drop even at the system limit
of 5 nA current, attesting the highly resistive nature of the pristine
substrates.
Atomic Force Microscopy
(AFM) and Scanning
Capacitance Microscopy (SCM)
As-grown AlN surface topographies
were assessed in a Bruker Dimenn class="Chemical">sion Icon AFM system with SiN tips
(Scanasyst-Air tips by Bruker, spring constant = 0.4 N/m). Topographic
data were acquired in the peakforce tapping mode and analyzed with
Nanoscope Analysis 1.9 and ImageJ[68] software.
For morphological quantification in Figure e, the 512 × 512 pixels in every image
were categorized based on their depth and those below a certain value
(threshold height, −ve) were considered to be part of a pit.
This way, shallow pits related to dislocations were excluded from
the analysis. The total areas occupied by the deeper pixels were then
normalized against the imaged areas and are presented as a measure
of noncoalescence. The maximum depth among all pixels in each image
was considered as the maximum probe depth.
SCM scans were carried
out on the cross section of specimens cleaved from the AlN-on-n class="Chemical">Si templates.
Preparing vertically abrupt sidewalls for examination, however, proved
to be impossible owing to the (111) orientation of the substrate.
Among all of the types, the sidewalls perpendicular to the ⟨110⟩
wafer notch were found to have the least surface tear and were chosen
for the scans. As-cleaved samples were first blown with purified N2 and then heated on a hot plate at 250 °C for 20 min
(ensuring minimal surface states in the native oxide). After soldering
a large indium ohmic contact on the Siside, the specimens were mounted
on a dedicated fixture with the Siside electrically contacting the
metallic chuck. The AFM was equipped with an SCM module for the measurements.
The used PtIr-coated doped Si tips (SCM-PIC-V2 from Bruker, spring
const. = 0.1 N/m) had a specified tip-radius of 25 nm, which is slightly
more than the distance between the acquired pixels (512 pixels in
10 μm). Thus, the spatial resolution is expected to be limited
by the distribution of the depletion region under the tip. In the
electrical configuration, the tip was kept grounded and all of the
biases were applied to the specimen through the chuck. The frequency
of the 0.5 VAC input signal was kept fixed at 90 kHz to allow only
the majority carriers to respond. Corresponding differential capacitance
was sensed as the change in the voltage output of a connected high-Q resonant circuit (f0 ∼
1 GHz). For each specimen, the lock-in phase (ϕL)
was optimized to offset the stray capacitances and to maximize the
SNR. Unless specified, no DC bias was applied. After the acquisition,
the data were analyzed with Nanoscope Analysis 1.9 and Gwyddion[69] software.
Coplanar
Waveguide (CPW) Fabrication and
Transmission Loss Measurement
Conventional photolithography
technique was used to fabricate identicn class="Chemical">al 50 Ω CPW transmission
lines[65] on top of the AlN-on-Si templates.
All of the samples were identically processed in the same batch, but
the metal layers were not optimized, which may have affected the absolute
magnitudes of the cumulative losses. Small-signal s-parameters of
the CPW lines were measured with ground-signal-ground probes while
mounted on a Cascade Summit 12000M station. Short–open–load–thru
(SOLT) calibration was performed before measurements using an off-wafer
impedance-standard-substrate (ISS). A Rhode and Schwarz ZVA-67 vector
network analyzer (VNA) was used for both calibration and measurements.
Scanning Transmission Electron Microscopy
(STEM) and Electron Energy Loss Spectroscopy (EELS)
Transmission
electron microscopy (TEM) lamellae (∼50 nm thin) were prepared
via focus ion beam milling un class="Gene">sing an FEI Helios equipped with a Ga
ion beam. STEM imaging in conventional dark-field (DF) and high-angle
annular dark-field (HAADF) modes were carried out in an FEI Tecnai
Osiris microscope equipped with a high-brightness XFEG source and
operated at 200 kV and an 80 pA beam current. EELS was performed with
Gatan’s Enfinium ER 977 (energy resolution ∼0.65 eV)
as the spectrometer in dual EELS mode measuring the zero-loss peak
and the low loss in the range of 45–255 eV. All of the EELS
micrographs were acquired with an electron beam convergence angle
of 11 mrad, an acceptance angle of 25 mrad, and a dwell time of 1
s/pixel with subpixel rastering.