low-temperature growth of gallium oxide thin films by
TRANSCRIPT
1
Low-temperature growth of gallium oxide thin films
by plasma-enhanced atomic layer deposition
Running title: Ga2O3 layers grown by PEALD
Running Authors: Mahmoodinezhad et al.
Ali Mahmoodinezhad,1 Christoph Janowitz,1 Franziska Naumann,2 Paul Plate,2 Hassan Gargouri,2 Karsten Henkel,1,3,a) Dieter Schmeißer,3 and Jan Ingo Flege1
1Applied Physics and Semiconductor Spectroscopy, Brandenburg University of Technology Cottbus–Senftenberg, K.-Zuse-Str. 1, 03046 Cottbus, Germany 2SENTECH Instruments GmbH, Schwarzschildstraße 2, 12489 Berlin, Germany 3Applied Physics and Sensor Technology, Brandenburg University of Technology Cottbus–Senftenberg, K.-Wachsmann-Allee 17, 03046 Cottbus, Germany
a) Electronic mail: [email protected]
Gallium oxide (Ga2O3) thin films were deposited by plasma-enhanced atomic layer deposition
applying a capacitively coupled plasma source where trimethylgallium (TMGa) as gallium
precursor and oxygen plasma (O2) were used in a substrate temperature (Ts) range of 80 to 200
°C. TMGa exhibits high vapor pressure and therefore facilitates the deposition at lower substrate
temperatures. The Ga2O3 films were characterized by spectroscopic ellipsometry (SE), X-ray
photoelectron spectroscopy (XPS), and capacitance–voltage (CV) measurements. The SE data
show linear thickness evolution with a growth rate of ~0.66 Å per cycle and inhomogeneity of ≤
2% for all samples. The refractive index of the Ga2O3 thin films is 1.86±0.01 (at 632.8 nm) and
independent of temperature whereas the bandgap slightly decreases from 4.68 eV at Ts of 80 °C
to 4.57 eV at 200 °C. XPS analysis revealed ideal stoichiometric gallium to oxygen ratios of 2:3
for the Ga2O3 layers with the lowest carbon contribution of ~10% for the sample prepared at 150
°C. The permittivity of the layers is 9.7±0.2 (at 10 kHz). In addition, fixed and mobile oxide
charge densities of 2 to 4 x 1012 and 1 to 2 x 1012 cm-2, respectively, were observed in the C-V
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characteristics. Moreover, the Ga2O3 films show breakdown fields in the range of 2.2 to 2.7
MV/cm. The excellent optical and electrical materials properties are maintained even at low
substrate temperatures as low as 80 °C. Hence, the TMGa/O2 PEALD process is suitable for
electronic and optoelectronic applications where low-temperature growth is required.
I. INTRODUCTION
Among the oxide dielectrics, Ga2O3 has gained tremendous interest in recent years due to
its outstanding materials properties, including, e.g., a wide bandgap (~5 eV)1, a high dielectric
constant2, a high break-down electric field (EBD)3, and a high thermodynamic stability4. Thin
films of Ga2O3 are nowadays widely used in numerous applications including high power and
high voltage field-effect transistors5, photovoltaics6, spintronics7, gate dielectric, and passivation
layers in III–V semiconductor-based devices to reduce the leakage current8-10. Owing to the
possibility to control the electrical conductivity between insulating and semiconducting
(typically n-type) behavior and because of its high optical transparency (~80%), Ga2O3 is a
promising candidate for transparent conducting oxides and thin film transistors11. In addition,
Ga2O3 exhibits gas dependent conducting behavior at elevated temperatures, making it one of the
most applicable materials for gas sensing12. To date, various approaches have been employed for
the deposition of Ga2O3 thin films such as chemical vapor deposition (CVD)7, molecular beam
epitaxy13, magnetron sputtering14, pulsed laser deposition4, and atomic layer deposition
(ALD)6,9,10,15-18.
Within the aforementioned deposition techniques, ALD with its inherent self-saturation
scenario is one of the most promising methods to get precise thickness control, excellent step
coverage, high conformality, and uniformity for the preparation of ultra-thin layers. The use of
plasma-enhanced ALD (PEALD) facilitates low-temperature deposition of high-quality films by
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increasing the rate of the (desired) chemical reaction while decreasing the interlayer diffusion
rate, thereby effectively broadening the ALD temperature window19. To date, different Ga
precursors were reported for the deposition of Ga2O3 in ALD and CVD processes, including
trimethylgallium (TMGa, [Ga(CH3)3])17, dimethylgallium isopropoxide9, and gallium(III)
isopropoxide (GTIP)10 in thermal ALD, TMGa20, [(CH3)2GaNH2]36, triethylgallium21, and
tris(2,2,6,6-tetramethyl-3,5-heptanedionato)gallium(III)22 in PEALD, and gallium
trishexafluoroacetylacetonate23, gallium(III) chloride24 in CVD. It should be noted that most of
these precursors could only be used at high temperature (> 300 °C) typically resulting in
undesired impurities within the films such as carbon and hydrogen, whose concentrations
strongly depend on the growth temperature. However, TMGa could be employed as a gallium
source at lower temperatures because it has a high vapor pressure and is highly volatile25, as
compared to other Ga precursors that require higher growth temperatures to obtain an
appropriate vapor pressure. Hence, a short pulse of TMGa could be adequate to quickly saturate
the surface reaction. Despite this obvious advantage, there are only a few studies about the
PEALD growth of Ga2O3 films using TMGa and O2 plasma20,26,27. Establishing this procedure
may thus pave the way for applications where low process temperatures are required. Also, from
a chemistry point of view, the similarity of TMGa to trimethylaluminum, which is commonly
used as Al source for the ALD of Al2O3 films28, may render this system a reference model for the
ALD of Ga2O3 films.
In this work, high-quality 10 and 30 nanometer thick gallium oxide layers were deposited
in the temperature window of 80 to 200 °C by PEALD where a capacitively coupled plasma
(CCP) source was applied. TMGa and oxygen plasma (O2) were used as gallium precursor and
oxidant co-reactant, respectively. The optical and electrical properties as well as the chemical
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composition of the Ga2O3 thin films were determined. The PEALD process delivered a constant
growth rate in the investigated substrate temperature range; the grown thin Ga2O3 films exhibited
an ideal gallium to oxygen (Ga:O) ratio with lowest carbon contamination for films prepared at
150 °C. Furthermore, the films show excellent optical and electrical properties exhibiting values
close to the ones of bulk crystalline material.
II. EXPERIMENTAL
A. Fabrication
The Ga2O3 thin films were deposited on 4″ n-type Si (100)/1.5 nm SiO2 substrates by
PEALD with alternating pulses of TMGa as Ga precursor and O2 plasma as co-reacting oxidant.
The deposition process was carried out at four different substrate temperatures (80, 100, 150 and
200 °C) in the SI ALD reactor (SENTECH Instruments GmbH)28 equipped with a laser
ellipsometer for in-situ ALD real-time monitoring (SENTECH, ALD Real Time Monitor). The
layers are expected to be amorphous in the investigated substrate temperature range.
High-purity N2 (99.999 %) was used as carrier gas of TMGa with a flow rate of 90 sccm.
During the plasma step the precursor line was closed and the nitrogen flow stopped. In this study,
the plasma was generated by a true remote CCP source in which the substrate is located apart
from the plasma generation area and caused neither high energy ions nor UV-light, which might
result in substrate surface damage. The employed CCP source, driven by a single radio frequency
of 13.56 MHz, is mounted to the upper flange of the reactor28,29; the plasma power and O2 (high
purity of 99.998 %) flow rate were set to 200 W and 150 sccm. One ALD cycle includes a 10 ms
pulse of TMGa followed by a purge pulse of 2 s, an oxygen plasma pulse of 5 s, and a 2 s purge
step. Figure 1 schematically shows the used PEALD pulse sequence.
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The samples are labeled as GaOz°C, where ‘z’ correspond to the substrate temperature
applied and GaO represents ‘gallium oxide’ without taking into account the elemental
composition.
FIG. 1. (Color online) Cycle sequence for the PEALD of Ga2O3 thin films. Each PEALD cycle
consisted of four sub-pulses with 10 ms TMGa vapor pulse (90 sccm N2 carrier gas), 2 s N2
purge pulse, 5 s (150 sccm, 200 W) O2 plasma and 2 s N2 purge pulse. The periodic deposition
cycle was repeated until the desired layer thickness was realized.
B. Characterization
The film thicknesses of the PEALD-Ga2O3 thin films were controlled using in-situ ALD-
RTM. This system allowed monitoring the short ALD cycles in the order of a few seconds with
high temporal resolution (20 ms) and a very high signal-to-noise ratio (δΔ = 0.01°,
Δ ellipsometric angle) at a single wavelength of 632.8 nm with incidence angle of 70°. Here, the
sample architecture was represented by a single, homogeneous film within a one-layer model.
The optical properties of the Ga2O3 thin films were investigated by spectroscopic ellipsometry
(SE) in different spectral ranges. UV/VIS/NIR measurements were performed with a SENTECH
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SER 850 in a wavelength range from 200 to 1000 nm at two incidence angles of 65° and 70°,
respectively. A Tauc-Lorentz oscillator was used for modeling and fitting the SE data to obtain
the film thickness, growth rate per cycle (GPC), refractive index, and optical bandgap of the
Ga2O3 layers. Furthermore, a 1.5 nm thick native oxide layer (SiO2) at the interface to the Si
substrate was considered in the analysis.
The chemical compositions and bonding states of the Ga2O3 films were determined by X-
ray photoelectron spectroscopy (XPS) using a hemispherical energy analyzer (Omicron EA 125)
with a dual anode X-ray source delivering Al Kα (1486.6 eV) as well as Mg Kα (1253.6 eV)
excitation. Prior to chemical analysis of the grown layers, the spectrometer transmission factor of
the analyzer was determined by investigating a Ga2O3 single crystal, cleaved under ultra-high
vacuum (UHV), in two different operation modes of the analyzer (constant analyzer energy
(CAE) and constant retarding ratio (CRR)) in accordance with Ref. 30. The photoelectrons were
collected at a take-off angle of 90° with regard to the sample surface plane to maximize the
sensitivity to the deeper layers while minimizing the contribution of surface contamination that is
inevitably present for ex-situ prepared samples. Nevertheless, to remove ambient adsorbates the
sample surface was sputtered by inert gas sputtering (Ar+, 2 keV, 4×10-6 mbar) applying a cold
cathode ion beam source (ISE 5, Scienta Omicron). The survey scan and high-resolution spectra
were collected with 50 and 20 eV pass energies with energy steps of 0.5 and 0.25 eV,
respectively. The obtained spectra were analyzed using CasaXPS analysis software to calculate
the atomic concentrations and gallium to oxygen (Ga:O) ratio by weighting the fitted peak areas
taking into account the respective atomic photoionization cross sections31 and the transmission
function of the analyzer30. In the peak fitting procedure a Gaussian/Lorentzian line shape, a
Shirley background subtraction, and a full width at half maximum (FWHM) of up to 1.7 eV were
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considered. It should be noted that in the high-resolution scans binding energy differences (ΔE ~
0.3±0.2 eV) for the core level signals (Ga3d, O1s and C1s) were observed pointing to a charging
effect that was reconsidered in the peak decomposition procedure. In order to calculate the
elemental compositions and Ga:O ratio before and after sputtering, the high-resolution core level
spectra (Ga3d, O1s, C1s) were collected using both Al Kα and Mg Kα excitation. To determine
the carbon contribution, Al Kα was used due to the fact that for this excitation neither Auger nor
satellite lines are perturbing the C1s main signal. On the contrary, Mg Kα was employed to
ascertain the Ga:O ratio because at this excitation the O1s core level region exhibits a single peak
without contributions of Auger or satellite lines. For the quantitative analysis, the Ga3d region at
lower binding energy was selected in order to collect electrons of higher kinetic energy
compared to the Ga2p region at higher binding energy, as the lower kinetic electrons of the Ga2p
levels deliver more surface sensitive information, which will still be more influenced by the
presence of surface contamination.
For the electrical measurements, metal–insulator–semiconductor (MIS) stacks were
prepared where the circular aluminum contacts (variable diameter between 300 and 800 µm)
were thermally evaporated through shadow masks on top of the Ga2O3/1.5nmSiO2/Si stack. The
stack sequence is illustrated in the lower inset of Fig. 10. For these measurements, thicker Ga2O3
layers of ~30 nm were employed to minimize the influence of probable leakage currents.
Capacitance-Voltage (C-V) measurements on these MIS structures were carried out with a LCR
meter Agilent 4284A.32 During one C-V loop the stack was biased from the inversion regime of
the semiconductor towards the accumulation counterpart and subsequently vice versa applying a
slow DC voltage ramp of 25 mV/s. The differential capacitance was recorded with a superposed
AC signal of 25 mV at frequencies of 1 MHz, 100 kHz, and 10 kHz. The C-V measurements
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were performed at different positions of the samples with varying contact pad areas. The
breakdown electrical field was determined from current-voltage measurements applying a
combination of Agilent E3649A power supply, HP34401 and PREMA4001 volt- and ammeters,
respectively.32
III. RESULTS AND DISCUSSION
A. Optical and spectroscopic characterization
Figure 2 shows the in-situ measurement of film thickness as a function of elapsed process
time for different substrate temperatures. The film thickness was obtained by modeling the
measured ellipsometric data with a one-layer model with a fixed refractive index of 1.86 (at
632.8 nm). A plot of the ellipsometric parameter delta (°) can be found in the supporting
information (Fig. S1). As typical for ALD, an increment and a reduction trend were observed in
the film thickness due to precursor adsorption and ligand removal. The measurement shows film
growth from the first cycle onwards where the nucleation behavior for all four samples is very
similar and linear film growth was achieved for all applied temperatures.
During opening the ALD line prior to the actual precursor pulse, the film thickness
increased. As soon as the precursor was dosed into the reactor, a second trend of increasing
thickness is witnessed. Remarkably, this double adsorption process was not observed during the
first cycle of the deposition of the films and occurs independent of substrate temperature. We
assume that due to its high volatility a certain amount of the precursor remained in the ALD line
after closing. When the ALD line was reopened and the flow of N2 carrier gas was restarted,
excess material was accidentally introduced into the reactor. Since the ALD lines were evacuated
before initiating the deposition process, this double adsorption does not take place during the
first cycle.
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FIG. 2. (Color online) Initial Ga2O3 film thickness evolution as a function of the process time for
different substrate temperatures within the PEALD process. The thickness was obtained by
modeling the in-situ ellipsometer data with a one-layer model with a constant refractive index of
1.86 (at 632.8 nm).
When investigating the plasma exposure step, upon plasma pulsing we observed an
abrupt reduction in film thickness; afterwards, saturation was attained within a few seconds.
During continuous plasma exposure the layer thickness remained constant, confirming that
neither undesirable film growth nor etching happened during this step.
Figure 3 illustrates the linear increase of the film thickness during PEALD process time
for all applied substrate temperatures. While almost no difference in the growth rate is visible
within the first 2000 s (film thickness of 10 nm), the slopes of the curves progressively deviate
with time up to a final thickness of 30 nm. This deviation results in a decrease of the GPC from
0.00
0.25
0.50
0.75
•
••
•
••
•
•
••
••
••
••
•
•
openning/closing of ALD line
0.00
0.25
0.50
0.75
•
••
•
••
••
•
•
•
•
•
•
•
•
•
•
TMGa (•)
Purge
Plasma
Purge
0.00
0.25
0.50
0.75
Th
ickn
ess [
nm
]
0 20 40 60 80 100
0.00
0.25
0.50
0.75
Time [s]
GaO200°C
GaO100°C
GaO150°C
GaO80°C
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0.70 Å/cycle (80 °C) to 0.63 Å/cycle (200 °C) as depicted in Fig. 4a. This phenomenon can be
explained by the reaction of the terminating hydroxyl groups forming a bridging oxygen
species33 as well as causing a decrease in film thickness and changes in nucleation behavior. This
well-known effect has been already reported for other materials systems like TiO2 (Ref. 34,35).
The achieved GPC (~0.66 Å/Cycle) for our Ga2O3 thin films is higher than that obtained for
other films deposited by the same PEALD process20.
FIG. 3. (Color online) Measured in-situ Ga2O3 film thickness versus prolonged process time up to
a total thickness of about 30 nm.
The optical properties of the as-deposited 30 nm Ga2O3 films were investigated by
considering the influence of various substrate temperatures. The GPC, refractive index,
thickness, inhomogeneity across the 4″ Si wafer (mapped at 69 positions) and the bandgap of the
layers were determined using the Tauc-Lorentz model to fit the SE data.
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The used process parameters lead to similar and very low inhomogeneity values in the
range of 1.5 to 2 % for all substrate temperatures as shown in Fig 4b. These low values indicate a
very good process control over large substrates (4″).
FIG. 4. (Color online) Growth rate (a) and inhomogeneity across a 4″ Si wafer (b) of the Ga2O3
layers depending on substrate temperature.
Fig. 5 shows the refractive index and the bandgap as a function of substrate temperature.
The refractive index and extinction coefficient in the full wavelength region are shown in the
supporting information (Fig. S2). The refractive index of the grown amorphous Ga2O3 films is
relatively constant (1.86±0.01 at 632.8 nm) in the investigated substrate temperature range. The
obtained refractive index value is in good agreement with other reported values using the same
PEALD process20,27 and is higher than values that have been achieved for thin films prepared by
other deposition methods, where values between ~1.6 and 1.8 (at a comparable wavelength) have
been reported36-38. The amorphous nature of as-deposited Ga2O3 layers might be one of the main
reasons why the refractive index remains nearly constant with increasing growth temperature.
80 100 120 140 160 180 2000
2
4
Inhom
og. [%
]
Substrate Temperature [°C]
0.60
0.65
0.70
GP
C [Å
/cycl.]
10 nm
30 nm
(b)
(a)
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The refractive index is dependent on the densification of material39,40; therefore, amorphous
films with low-density might be prone to air trapping in the layer’s pores leading to an effective
reduction of the refractive index (when compared to post-annealed samples reported in
literature6). However, in the investigated substrate temperature range we do not expect any
significant change in the amorphous nature of our samples, consequently resulting in an almost
constant refractive index.
The bandgap slightly decreases with increasing substrate temperature. Taking into
account the error bars of the measurement, the deviation is, however, in the range of ~100 meV.
In this respect, our finding is in agreement with data of Choi et al.10, where no significant
changes of the bandgap in the temperature range of 150 to 250 °C were observed for layers
prepared by thermal ALD using GTIP and water. The obtained optical bandgap of 4.63±0.05 eV
is slightly lower than other values (4.8eV at Ts =200°C) reported in literature for the same
PEALD process26. This fact could be attributed to the amorphous phase of the as-deposited
Ga2O3 films.
A summary of the obtained optical properties can be found in Table I.
In order to avoid charging effects during the XPS measurements, Ga2O3 film of 10 nm
film thickness were prepared using the same process parameters. The achieved growth rates and
inhomogeneities for these samples can be found in the supporting information (Table S1). We
assume that the optical properties obtained from the 30 nm thick films translate to their thinner
counterparts.
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FIG. 5. (Color online) SE model results of the optical band gap and refractive index as a function
of deposition temperature for gallium oxide samples. The measurements were carried out ex-situ
on 30 nm thick samples.
TABLE I. Summary of main determined properties of the Ga2O3 layers characterized in this study.
The tabulated parameters are substrate temperature (Ts), GPC, inhomogeneity (inhomog.) across
4″ Si wafers, refractive index (n), optical energy gap (Eg), Ga:O ratio, C1s concentration,
permittivity (k) at 10 kHz, negative fixed charges (Nfix), and electrical breakdown field (EBD).
The Ga:O ratio and C1s contribution were determined from 10 nm thick films whereas all other
properties were obtained from 30 nm thick layers.
Samples Ts
[°C]
GPC
[Å/cycle]
inhomog.
[%]
n
[@632.8nm]
Eg
[eV]
Ga:O C1s
[%]
k
[@10kHz]
Nfix
[1012cm-2]
EBD
[MV/cm]
GaO80°C
GaO100°C
GaO150°C
GaO200°C
80
100
150
200
0.70
0.67
0.66
0.63
1.6
1.8
1.6
2.0
1.85±0.005
1.85±0.003
1.86±0.004
1.87±0.006
4.68±0.02
4.66±0.03
4.61±0.02
4.57±0.02
0.67
0.65
0.66
0.67
12.2
12.6
10.6
15.9
9.8±0.1
9.4±0.2
9.6±0.1
9.9±0.2
-3.8±0.1
-3.1±0.2
-2.1±0.1
-2.2±0.1
2.2±0.3
2.4±0.2
2.7±0.3
2.4±0.3
80 100 120 140 160 180 2004.0
4.2
4.4
4.6
4.8
Ba
nd
ga
p [
eV
]
Substrate temperature [°C]
t = 31.5 0.4 nm
1.82
1.83
1.84
1.85
1.86
1.87
1.88
1.89
1.90
1.91
1.92
n @
63
2.8
nm
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The atomic composition of the Ga2O3 thin films was determined using XPS. Figure 6
shows the survey spectra of the as-deposited samples. Obviously, the spectra contain the
expected photoemission lines of Ga (Ga2p, Ga3s, Ga3p, Ga3d, GaLMM Auger) and oxygen
(O1s, O2s, OKLL Auger), but also of carbon (C1s, CKVV Auger)9,23,38,41-43.
FIG. 6. (Color online) XPS survey spectra of the as-deposited Ga2O3-PEALD thin films prepared
at different substrate temperatures as indicated. The spectra were recorded with Mg Kα
excitation.
The C1s signals imply that carbon was adsorbed on the sample surface during their
transfer for ex-situ XPS analysis. Therefore, all as-deposited samples were exposed to Ar+ ion
beam sputtering for one minute to remove the surface contamination. The Ga:O ratio deduced
from Ga3d and O 1s core level data as well as the carbon concentrations (C1s data) before and
after sputtering are depicted versus the PEALD substrate temperature in Fig. 7; the values of the
sputtered samples are additionally given in Table I. Remarkably, the Ga:O ratio is very close to
the ideal value of 2:3 for all investigated samples. In other works using the same PEALD process
higher deviations (0.70 and 0.77 for as-deposited and annealed (900°C) films) from that ideal
1000 800 600 400 200 0
GaO200°C
Mg K
GaO150°C
C K
VVIn
ten
sity [
arb
. u
nits]
Binding energy [eV]G
a 2
p1/2
Ga 2
p3/2
O K
LL
O 1
s
Ga L
MM
C 1
s
Ga
3s
Ga
3p
Ga 3
d,
O 2
s
GaO80°C
GaO100°C
Survey Spectra Ga2O
3
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value were observed.27 Obviously, the carbon concentration is significantly decreased after
sputtering, where it is nearly constant (C1s ~ 12.4±0.2%) within the Ts range of 80 to 100 °C.
The lowest and highest values are found at Ts = 150 °C (C1s ~ 10.6±0.1%) and Ts = 200 °C (C1s
= ~ 15.9±0.1%), respectively.
FIG. 7. (Color online) Gallium to oxygen ratio (a) and carbon contamination (b) of the Ga2O3
films vs. substrate temperature.
Figure 8 shows the decomposition of the Ga3d spectra into four sub-peaks after
calibrating the binding energy (BE) of the main (Ga-O) component to 20.5 eV. The appearance
of the highly intense peak confirms the presence of Ga-O bonds, i.e., the formation of a Ga2O3
thin film20,21. A weak peak at higher BE (24.2±0.1 eV) is identified as the O2s core level42,44.
Therefore, this O2s contribution might slightly impact the Ga3d raw area leading to an
overestimation of the Ga atomic concentration, however we expect that this error is small (≤2%).
The two further sub-peaks on the higher and lower BE shoulders of the Ga-O peak (22.5±0.1 eV
and 19±0.1 eV) are attributed to carbonates and Ga-OH species44. The relative intensities of the
0.60
0.65
0.70
0.75
(b)
Al K
Ga3d
/O1s r
atio
ideal
1 min sputtering
as-deposited
Mg K
(a)
80 100 120 140 160 180 2009
12
15
18
21
C1s [%
]
Substrate temperature [°C]
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different Ga3d components are listed in Table II and remain essentially constant with substrate
temperature; just the hydroxide contribution is slightly higher at Ts = 80 °C and is consistently
getting smaller with increasing substrate temperature, possibly owing to the lower thermal
stability of the hydroxide species.
FIG. 8. (Color online) Ga 3d core level XPS data (Mg Kα) of Ga2O3 layers grown at substrate
temperatures of (a) 80 °C, (b) 100 °C, (c) 150 °C, and (d) 200 °C and their decomposition.
Analogously, the O1s core level XPS spectra were fitted into four discrete peaks (Fig. 9)
upon calibrating the BE to 531 eV. This sharp peak corresponds to Ga-O bonding similar to the
Ga3d spectra20,21,38,45,46. Two weak peaks at 532.8±0.1 eV and 529.5±0.2 eV) are attributed to O-
H bonds and O1s satellite peak, respectively. Furthermore, the peak located at 531.6±0.1 eV
points to oxygen bonded with carbon (O-C)43,47,48. The contributions of these sub-peaks in the
0
1
1min sputtering
0
1
0
1
No
rma
lize
d in
ten
sity
26 24 22 20 18
0
1GaO200°C
GaO150°C
GaO100°C
Mg K
Binding energy [eV]
Ga-OHO 2s
d)
c)
b)
a)
data
⎯⎯ fit
carbonates
Ga 3d
GaO80°CGa−O
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O1s core level are also given in Table II. Similarly to the Ga3d decomposition data, with
increasing substrate temperature the contributions of both carbonyl (oxygen bonded to carbon)
and hydroxyl (oxygen bonded to hydrogen) groups tend to decrease except for Ts = 100 °C where
particularly a strong increase of the carbonyl contribution is observed. It was found that the film
grown at 150 °C exhibits the lowest total carbon (Table I) and carbonyl concentrations in the
O1s region (Table II) as well as it is in the lower carbonate concentration range as derived from
the Ga3d data (Table II) among all our samples.
FIG. 9. (Color online) O1s core level XPS data of Ga2O3 layers deposited at substrate
temperatures of (a) 80 °C, (b) 100 °C, (c) 150 °C, and (d) 200 °C and their decomposition.
0
1
0
1
0
1
O (satellite)
No
rma
lize
d in
ten
sity
Mg K
Ga−O
536 534 532 530 528
0
1 GaO200°C
GaO150°C
GaO100°C
Binding energy [eV]
O−CO−H
1min sputtering
d)
c)
b)
a)
data
⎯⎯ fit
O 1s
GaO80°C
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TABLE II. Relative sub-peak intensities in the Ga3d and O1s core level XPS spectra of Ga2O3
PEALD films.
Ga3d O1s
Samples carbonates% Ga-O% Ga-OH% O-H% O-C% Ga-O%
GaO80°C
GaO100°C
GaO150°C
GaO200°C
6.3
5.7
5.8
5.7
76.9
79
78.8
79.7
12.6
11.4
11.3
10.9
5.7
7.8
7.2
6.1
21.8
32.2
16.5
19.1
68.1
55
72.6
70.7
B. C-V characterization
In this section the C-V data of the Ga2O3 PEALD samples are compared. Figure 10
exemplarily depicts the C-V measurements at 10 kHz for the GaO80°C sample for different
contact areas.
FIG. 10. (Color online) C-V measurements of the sample GaO80°C at different contact pad
diameters () as listed beside each curve. The measurement direction is indicated by the arrows.
The lower inset illustrates the MIS stack sequence; the upper inset shows one C-V loop at 1 MHz
( = 500 µm).
0 1 2 3 4
0.0
0.2
0.4
0.6
0.8
1.0
n-Si
1.5 nm SiO2
30 nm Ga2O3
Al2
300
400
500
600
GaO80°C
10 kHz
Ca
pa
cita
nce
[n
F]
Voltage [V]
[µm]
700
1
0 2 4
0
11 MHz
1
2
No
rm.
ca
p.
Voltage [V]
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The C-V data follow the typical behavior for an n-type semiconductor. Also, the expected
scaling of the accumulation capacitance Cacc with the device dimension (contact area) is visible.
However, we also find positive flat-band voltage (VFB) shifts as well as hysteresis effects within
the measurements. The latter is significantly present in the first-time measurement on each
contact, which was carried out at 1 MHz; an example is given in the upper inset of Fig. 10. This
phenomenon will be discussed below.
To determine the permittivity of the Ga2O3 layers, the accumulation capacitances of the
C-V loops determined for different contact areas (A) were normalized and plotted against A (Fig.
11). For this procedure, we chose the C-V data recorded at 10 to 100 kHz to avoid influences of
series resistances on Cacc at higher frequencies. Assuming a combination of two capacitances
(representing the Ga2O3 film and the interfacial SiO2) connected in series, the following equation
can be developed:
A
kd
d
k
dC
SiOOGa
SiO
OGa
OGaacc*
11
1*
232
2
32
32
0 +
=
(1)
where dGa2O3, kGa2O3, dSiO2 (1.5 nm, as modeled in the ellipsometric data – see above), and kSiO2
(3.9) denote the thickness and relative permittivity of the Ga2O3 and the interfacial SiO2 layers,
respectively, and ε0 the vacuum permittivity (cf. Refs. 28, 49 for further details).
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FIG. 11. (Color online) Normalized Cacc against contact area according to Eq. (1) for the samples
GaO80°C, GaO100°C, GaO150°C, and GaO200°C as indicated in the legend. The linear fits used for the
determination of the permittivity are drawn with the corresponding colors. The data are shown
for C-V measurements recorded at 10 kHz.
In Fig. 11, the 10 kHz data are plotted following Eq. (1). Subsequently, these data were
linearly fitted in accordance with Eq. (1); the permittivity kGa2O3 was then deduced from the
slope of the linear fit.
In the investigated substrate temperature range we found just a slight variation of the
permittivity with values of 9.6±0.3 in the frequency range of 10 to 100 kHz (Fig. 12a). Only for
the GaO100°C sample the permittivity is noticeably lower than for the other three samples.
Between 100 °C and 200 °C a slight increase in permittivity with temperature is identified,
consistent with the optical data, where a slight increase of the refractive index with temperature
was observed (see above). Our Ga2O3 layers show similar permittivity values as observed for
thermal ALD and PEALD layers prepared with GTIP and water10 or [(CH3)2GaNH2]3 and
oxygen plasma6. For annealed (700-900°C), crystalline samples fabricated also in the TMGa/O2
plasma process much lower values were reported so far (5 to 5.4 at 1 MHz)27.
0.0 0.1 0.2 0.3 0.40.0
0.5
1.0
1.5
2.0
2.5
3.0
3.5
4.0
GaO80°C
GaO100°C
GaO150°C
GaO200°C
Contact area [mm2]
Cacc*d
Ga
2O
3
/0 [
mm
2]
10kHzTh
is is
the au
thor’s
peer
revie
wed,
acce
pted m
anus
cript.
How
ever
, the o
nline
versi
on of
reco
rd w
ill be
diffe
rent
from
this v
ersio
n onc
e it h
as be
en co
pyed
ited a
nd ty
pese
t.PL
EASE
CIT
E TH
IS A
RTIC
LE A
S DO
I: 10
.1116
/1.51
3480
0
21
FIG. 12. (Color online) Permittivity (a) at 10 (red open circles) and 100 kHz (blue filled squares)
as well as (b) negative fixed (green open squares) and mobile (black filled triangles) charges
(deduced from C-V measurements at 1 MHz) against substrate temperature of the PEALD
processed Ga2O3 samples.
Recently, Fiedler et al. investigated the static dielectric constant of β-Ga2O3 in
dependence of the principal planes and found an average value over all orientations of
11.2±0.2.50 The authors argued that lower values are observed for amorphous or polycrystalline
80 100 120 140 160 180 2000
1
2
3
4
b)
neg. fixed
mobile
Ch
arg
es [
10
12 c
m-2]
8
10
12
100kHz
10kHz
Substrate temperature [°C]
Pe
rmittivity
a)
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layers since the crystalline network is more densely packed than the amorphous phase.50
According to the Clausius-Mossotti equation51, this densification is accompanied by a higher
relative dielectric constant for the crystalline phase. However, we expect our layers, which were
prepared at temperatures of 200 °C and below, to be amorphous as also confirmed by Ref. 20.
The abovementioned flat-band voltage shifts and hysteresis effects within the C-V loops
are observed for all investigated samples. Thereby, the first-time measurement on every contact
pad performed at 1 MHz showed the highest hysteresis, afterwards it was reduced as can be seen
when comparing the data in the main panel (mostly third measurement - at 10 kHz) and upper
inset (first measurement) in Fig. 10. This reduction of the hysteresis is not due to the change of
the measurement frequency as it was proven by repeated measurements at 1 MHz on selected
contacts (supporting information Fig. S3), where a reduction of the hysteresis was observed as
well, when the first-time and subsequent C-V loops were compared at this frequency. However,
this hysteresis reduction is accompanied by a further positive flat-band voltage shift in such a
way that the subsequent C-V loop is located close to the reverse branch of the first-time C-V
loop (labeled “2” in the upper inset of Fig. 10). Afterwards, i.e., in further subsequent C-V loops,
the C-V characteristics remained constant.
Typically, shifts of positive flat-band voltage point to negative fixed charges inside the
insulator.52 Similar behavior was observed for Ga2O3 layers prepared in PEALD processes using
TMGa27 or [(CH3)2GaNH2]3 (Ref. 53) and oxygen plasma. Liu et al. speculated about oxygen
vacancy formation due to a SiO2 interfacial layer between Si and Ga2O3, finally causing extra
negative charges.53 We have recently discussed the electronic structure of Ga2O3 containing
intrinsic defect states, namely polaronic, excitonic and charge transfer states, formed by mixed
atomic valence states.54 In this picture we developed a model where the excitonic states are states
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that are “easy to be filled/refilled” as they are located close to the Fermi level; conversely, charge
transfer states are highly localized and related to fixed charges.55 Initially, the charge transfer
states and hence the fixed negative charges are created by the PEALD process (it should be noted
that these intrinsic electronic defect states are also existent in single crystals; however, their
abundance depends on the preparation conditions54,55). During the first C-V loop, applying a
positive voltage drives the semiconductor into accumulation. Hence, a large reservoir of
electrons is available at the Ga2O3/Si interface that will be injected into the insulator and trapped
in the charge transfer states leading to an increased positive flat-band voltage position in the C-V
reversed scan (labeled by “2” in Fig. 10). Subsequently applying a negative voltage inside the C-
V loop is not sufficient to depopulate these states again. Therefore, in the next C-V run these
states cannot be filled again, resulting in the location of the C-V loop close to the branch labeled
with “2” in Fig. 10. Ideally, after completion of the charge transfer process the C-V loop should
exhibit no hysteresis, but still, electrons can easily be trapped in and released from the excitonic
defect states since they are located close to the Fermi level, causing the remaining C-V hysteresis
as displayed in the main panel of Fig. 10 as well as in the supporting information (Fig. S3).
To determine the concentration of initially fixed (Nfix) and ‘hysteretic’ (Nhyst) charges, the
first-time C-V measurements at 1 MHz were analyzed. The ideal work function difference of the
metal electrode and the semiconductor substrate ΦMS (-0.1 eV) was calculated assuming the
aluminum work function and silicon electron affinity of 4.2 eV56 and 4.05 eV57, and determining
the semiconductor Fermi level position (0.245 eV below the conduction band minimum) from
the substrate doping (2.8±1.5 × 1015 cm-3, i.e., 1 to 3.5 Ωcm) calculated via the depletion
approximation57 for the 1 MHz C-V data. The MIS flat-band capacitance was calculated using This
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the semiconductor substrate doping level57 and Cacc; this value was then used to determine the
flat-band voltage in the 1 MHz C-V data. Finally, Nfix and Nhyst were deduced via
Nfix = (ΦMS / e-VFB) * Cacc / A (2a)
Nhyst = ΔVFB * Cacc / A, (2b)
respectively, where e is the elementary charge.
Fig. 12b shows the resulting Nfix and Nhyst values depending on PEALD substrate
temperature. Nhyst is relatively constant (~ 1×1012 cm-2) with substrate temperature, just for the
GaO100°C sample it is higher (1.9 × 1012 cm-2). Generally, Nfix shows a trend to diminish with
increasing substrate temperature. At 80 °C, it amounts to about 4 × 1012 cm-2; at 150 °C, it
exhibits a minimum of about 2 × 1012 cm-2. The latter value is similar to what has been observed
in other works using the same PEALD process, but following post deposition annealing.27
Combining both XPS and electrical data, we may draw the following two conclusions on
how the specific choice of PEALD process parameters influences the resulting materials
properties. Firstly, at lower Ts (80 to 100 °C) the layers have a higher number of fixed and/or
hysteretic charges than at higher Ts (150 to 200 °C). Comparing the carbonate and carbonyl
contributions in the Ga3d and O1s XPS data (Table II), respectively, these amounts are also
higher in sum at lower Ts than at higher Ts. Hence, we speculate that there exists a correlation
between carbon within the layers and the fixed and mobile charges, suggesting that carbon might
act as a trap center. However, further investigations such as temperature-dependent current-
voltage and deep-level transient spectroscopy measurements are needed to clarify this issue,
which are beyond the scope of the current work. Particularly, the mentioned correlation holds for
the GaO150°C film, which exhibits the lowest total carbon amount (Table I) and the lowest
carbonyl contribution in the O1s data (Table II) as well as the lowest Nfix (Table I). In case Nfix
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and Nhyst should be minimized for the desired application of the Ga2O3 layer, the higher Ts
temperature range (150 to 200 °C) should be chosen. Conversely, a post deposition annealing
step might be reasonable for the reduction of Nfix and Nhyst. This, however, is not applicable when
low process temperatures are required. Recently, we have demonstrated for aluminum nitride
PEALD layers that the specific choice of plasma source might also be an option to influence Nhyst
and Nfix, where we obtained reduced values when using an inductively coupled plasma source
instead of a CCP source (which was also applied in the current work).58 This finding implies that
further tuning of the electrical materials properties of the Ga2O3 films should readily be feasible.
Secondly, the GaO100°C sample with the highest Nhyst exhibits the lowest permittivity
value. Furthermore, this sample shows the highest (albeit small) deviation of the Ga:O ratio from
the ideal value (oxygen-rich, see Fig. 7), which might be caused by the higher concentration of
O–C and O–H bonds in the O1s data of this sample (Fig. 9b and Table II). Therefore, the
polarizability and hence the permittivity (according to the Clausius-Mossotti equation50) of the
material seem to be affected by the concentration of injected charges as well as by changes in the
concentration of local dipoles and their polarizabilty.
Furthermore, the electrical breakdown field EBD was determined; the achieved values are
also given in Table I. Here, values between 2.2 and 2.7 MV/cm were identified. The theoretical
breakdown field for β–Ga2O3 is expected to be 8 MV/cm4,5; however, the typically achieved
experimental values are far below this value11. The breakdown electric field values of our
amorphous layers are similar to those reported for electron beam evaporated59 and
photoelectrochemically deposited60 thin films, where values of 2.1 and 2.8 MV/cm were
obtained, respectively. As-grown PEALD layers prepared with [(CH3)2GaNH2]3 and O2 plasma
have shown very leaky behavior; high-temperature (Ts ≥ 700 °C) rapid thermal post-deposition
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annealing was necessary to decrease the leakage current significantly, but the breakdown field
was only about 1 MV/cm.6 Therefore, a further improvement in the insulating behavior of our
layers may be expected when a PDA step is compatible with the desired process conditions. It
should be noted that higher breakdown fields have recently been observed for amorphous layers
prepared by thermal ALD (6.5 to 7.6 MV/cm at Ts between 150 and 250 °C using GTIP and
water)10 as well as by PEALD (6.8 MV/cm at Ts = 200°C and plasma power of 200 W) applying
TMGa and an O2 plasma.26
IV. SUMMARY AND CONCLUSIONS
This paper documents the optical and electrical properties as well as the chemical
composition of amorphous Ga2O3 thin films deposited by PEALD on Si(100) substrates with
TMGa and O2 plasma in the Ts range of 80 to 200 °C. From ellipsometry a constant growth rate
of ~0.66 Å/cycle is inferred; the refractive index and optical bandgap amount to 1.86±0.01 and
4.63±0.05 eV, respectively. Further, the SE data confirm that the chosen substrate temperature
range lies within the ALD window. The XPS results proved that all samples have an almost ideal
gallium to oxygen ratio of 2:3. The lowest carbon contamination (~10%) is observed at Ts = 150
°C. The high-resolution Ga3d and O1s core level spectra corroborated the overwhelming
presence of Ga-O bonds in the films, whose fraction increases with increasing temperature while
the concentration of carbonates, carbonyl, and hydroxide species decreases. The C-V data
revealed a dielectric constant of 9.7±0.2 at frequency of 10 kHz for the Ga2O3 films. Moreover,
fixed and mobile oxide charge densities of 2 to 4 x 1012 and 1 to 2 x 1012 cm-2 were found. In
addition, the breakdown electric field lies within the range of 2.2 to 2.7 MV/cm, with the highest
value obtained at 150 °C. Summarizing all data, the sample prepared at Ts = 150 °C carries the
best performance. Remarkably, their excellent optical and electrical materials properties do not
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significantly change even at substrate temperatures as low as 80 °C, rendering our Ga2O3 thin
films very well suited for electronic and optoelectronic applications where low-temperature
growth is required.
ACKNOWLEDGMENTS
This work is financially supported by the Federal Ministry for Economic Affairs and Energy
(BMWi) of Germany within the ZIM program (ZF4510602AG7, ZF4245503AG7). A.M.
acknowledges the funding by the Graduate Research School (GRS) of the Brandenburg
University of Technology Cottbus–Senftenberg within the Cluster »Functional Materials and
Film Systems for Efficient Energy Conversion (FuSion)«. We acknowledge Guido Beuckert for
technical support.
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TABLES
TABLE I. Summary of main determined properties of the Ga2O3 layers characterized in this study.
The tabulated parameters are substrate temperature (Ts), GPC, inhomogeneity (inhomog.) across
4″ Si wafers, refractive index (n), optical energy gap (Eg), Ga:O ratio, C1s concentration,
permittivity (k) at 10 kHz, negative fixed charges (Nfix), and electrical breakdown field (EBD).
The Ga:O ratio and C1s contribution were determined from 10 nm thick films whereas all other
properties were obtained from 30 nm thick layers.
Samples Ts
[°C]
GPC
[Å/cycle]
inhomog.
[%]
n
[@632.8nm]
Eg
[eV]
Ga:O C1s
[%]
k
[@10kHz]
Nfix
[1012cm-2]
EBD
[MV/cm]
GaO80°C
GaO100°C
GaO150°C
GaO200°C
80
100
150
200
0.70
0.67
0.66
0.63
1.6
1.8
1.6
2.0
1.85±0.005
1.85±0.003
1.86±0.004
1.87±0.006
4.68±0.02
4.66±0.03
4.61±0.02
4.57±0.02
0.67
0.65
0.66
0.67
12.2
12.6
10.6
15.9
9.8±0.1
9.4±0.2
9.6±0.1
9.9±0.2
-3.8±0.1
-3.1±0.2
-2.1±0.1
-2.2±0.1
2.2±0.3
2.4±0.2
2.7±0.3
2.4±0.3
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TABLE II. Relative sub-peak intensities in the Ga3d and O1s core level XPS spectra of Ga2O3
PEALD films.
Ga3d O1s
Samples carbonates% Ga-O% Ga-OH% O-H% O-C% Ga-O%
GaO80°C
GaO100°C
GaO150°C
GaO200°C
6.3
5.7
5.8
5.7
76.9
79
78.8
79.7
12.6
11.4
11.3
10.9
5.7
7.8
7.2
6.1
21.8
32.2
16.5
19.1
68.1
55
72.6
70.7
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FIGURE CAPTIONS
FIG. 1. (Color online) Cycle sequence for the PEALD of Ga2O3 thin films. Each PEALD cycle
consisted of four sub-pulses with 10 ms TMGa vapor pulse (90 sccm N2 carrier gas), 2 s N2
purge pulse, 5 s (150 sccm, 200 W) O2 plasma and 2 s N2 purge pulse. The periodic deposition
cycle was repeated until the desired layer thickness was realized.
FIG. 2. (Color online) Initial Ga2O3 film thickness evolution as a function of the process time for
different substrate temperatures within the PEALD process. The thickness was obtained by
modeling the in-situ ellipsometer data with a one-layer model with a constant refractive index of
1.86 (at 632.8 nm).
FIG. 3. (Color online) Measured in-situ Ga2O3 film thickness versus prolonged process time up to
a total thickness of about 30 nm.
FIG. 4. (Color online) Growth rate (a) and inhomogeneity across a 4″ Si wafer (b) of the Ga2O3
layers depending on substrate temperature.
FIG. 5. (Color online) SE model results of the optical band gap and refractive index as a function
of deposition temperature for gallium oxide samples. The measurements were carried out ex-situ
on 30 nm thick samples.
FIG. 6. (Color online) XPS survey spectra of the as-deposited Ga2O3-PEALD thin films prepared
at different substrate temperatures as indicated. The spectra were recorded with Mg Kα
excitation.
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FIG. 7. (Color online) Gallium to oxygen ratio (a) and carbon contamination (b) of the Ga2O3
films vs. substrate temperature.
FIG. 8. (Color online) Ga 3d core level XPS data (Mg Kα) of Ga2O3 layers grown at substrate
temperatures of (a) 80 °C, (b) 100 °C, (c) 150 °C, and (d) 200 °C and their decomposition.
FIG. 9. (Color online) O1s core level XPS data of Ga2O3 layers deposited at substrate
temperatures of (a) 80 °C, (b) 100 °C, (c) 150 °C, and (d) 200 °C and their decomposition.
FIG. 10. (Color online) C-V measurements of the sample GaO80°C at different contact pad
diameters () as listed beside each curve. The measurement direction is indicated by the arrows.
The lower inset illustrates the MIS stack sequence; the upper inset shows one C-V loop at 1 MHz
( = 500 µm).
FIG. 11. (Color online) Normalized Cacc against contact area according to Eq. (1) for the samples
GaO80°C, GaO100°C, GaO150°C, and GaO200°C as indicated in the legend. The linear fits used for the
determination of the permittivity are drawn with the corresponding colors. The data are shown
for C-V measurements recorded at 10 kHz.
FIG. 12. (Color online) Permittivity (a) at 10 (red open circles) and 100 kHz (blue filled squares)
as well as (b) negative fixed (green open squares) and mobile (black filled triangles) charges
(deduced from C-V measurements at 1 MHz) against substrate temperature of the PEALD
processed Ga2O3 samples.
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uscri
pt. H
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e onli
ne ve
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10.11
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5134
800
This
is the
autho
r’s pe
er re
viewe
d, ac
cepte
d man
uscri
pt. H
owev
er, th
e onli
ne ve
rsion
of re
cord
will
be di
ffere
nt fro
m thi
s ver
sion o
nce i
t has
been
copy
edite
d and
type
set.
PLEA
SE C
ITE
THIS
ART
ICLE
AS
DOI:
10.11
16/1.
5134
800