spectroscopic ellipsometry for in situ applications...spectroscopic ellipsometry is a useful...
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© 2019 J.A. Woollam jawoollam.com 1
Greg PribilApplications Engineer
Spectroscopic Ellipsometry for In Situ Applications
Harvard University, NNCI ALD/MOCVD/MBE Symposium – October 2019
© 2019 J.A. Woollam jawoollam.com 2
Outline
Spectroscopic Ellipsometry (SE) Introduction
In Situ SE Integration and Common Considerations
In Situ SE Examples
© 2019 J.A. Woollam www.jawoollam.com 3
Founded in 1987 by Prof. John A. Woollam based on
spin-off of research at University of Nebraska-Lincoln.
> 60 employees
> 190 patents
J.A. Woollam Co. History
© 2019 J.A. Woollam www.jawoollam.com 4
What is Polarization? Describes shape of Electric Field relative to direction of travel.
Linear: arbitrary amplitudes, in-phase Circular: equal amplitudes, 90° phase difference Elliptical: arbitrary amplitudes, arbitrary phases
X
Y
Z
wave1
wave2
© 2019 J.A. Woollam jawoollam.com 5
Spectroscopic Ellipsometry (SE)
SE measures the change of
polarization as light interacts
with a thin film coated surface
Coherent interference occurs when
light recombines after traveling
different paths through thin film
t
2~n
1~n
0~n
© 2019 J.A. Woollam jawoollam.com 6
What Can SE Determine?
© 2019 J.A. Woollam jawoollam.com 7
In Situ Ellipsometry Real-time monitoring and control
Complete sample history
– Before, during and after process
Direct measurement of surfaces & interfaces
Atomic Layer
Deposition
J.N. Hilfiker “In situ spectroscopic ellipsometry
(SE) for characterization of thin film growth”,
chapter in In situ characterization of thin film
growth, G. Koster and G. Rijnders, eds.,
Woodhead Publishing: Cambridge, UK (2011)
© 2019 J.A. Woollam jawoollam.com 8
In Situ Spectroscopic Ellipsometry Source and Receiver attach to standard window flanges on
process chamber for non-invasive, non-contact measurements.
CCD detection: Possible to measure
>1000 wavelengths from UV to NIR –
collected multiple times each second.
High Sensitivity to Thin Film properties:
Thicknesses from <1nm to 10+ microns.
Measurement is ratio, so accurate
with fluctuating intensity due to
window coating, moving sample,
etc.
© 2019 J.A. Woollam jawoollam.com 9
In Situ Spectroscopic Ellipsometry Data
Spectral Datastudy sample
before, during, &
after film growth
Dynamic
SE Datacontains
continuous
Spectral Data
Time in Minutes
Me
asu
red
Yin
deg
rees
200 1000
0
15
30
45
60
75
90
90
00 8
Wavelength in nm
45
75
60
30
15
Yin
deg
rees
© 2019 J.A. Woollam jawoollam.com 10
CompleteEASE User Interface In situ Tab: Analysis Tab: Measurement Tab:
“Custom” tabs (e.g., Heat Cell)
Optical Models: Gen-Osc
B-Spline
Cauchy …
© 2019 J.A. Woollam jawoollam.com 11
Application: Thickness and Growth Rate
Most common in situ SE application:
Real-Time film thickness.
Film thickness and growth rate shown
for sputter deposition of SiO2 thin film.
9.9 10.2 10.5 10.8 11.1 11.4 11.7
Time in Minutes
400
500
600
Layer
thic
kness in
Å
Target thickness
Shutter close
time
SE data
points
Thickness control algorithm for
precise process control.
Controlled growth shown for a 583Å
GaAs thin film.
© 2019 J.A. Woollam jawoollam.com 12
Advantages of Spectroscopic Ellipsometers
Die
lectr
ic f
unction
Die
lectr
ic f
unction
Langereis et al., J. Phys. D: Appl. Phys. 42, 073001 (2009)
Wide spectral range
– Near IR range for conductive film
– UV range for semiconductors and
dielectrics
No gaps in spectrum
– Interference enhancement to study thin
metal films
Software with extensive modeling
options for most-general samples
– General Oscillator models
• Drude for conductivity
• Tauc-Lorentz for amorphous materials
• Parameterized semiconductor models
• ....
– B-spline parameterizations
© 2019 J.A. Woollam jawoollam.com 13
Chamber Integration Requires optical access to the Sample
during measurement.
SE measurements can be continuous,
periodic, or triggered.
SE measurement angle defined from
sample normal to ellipsometer viewport.
– Source Angle = Receiver Angle
– Typical “default” port angle ~ 70°,
with most chambers designed for port
angle between 60° to 75°.
Source Unit
Source Stage
Receiver Unit
Receiver Stage
Viewport
(Window)Viewport
(Window)
Angle
© 2019 J.A. Woollam jawoollam.com 14
Examples: In Situ/In-Line SE Implementations
Moving metal s
heet
Ellipsometer housed in single unit to protect from harsh industrial environment.
Double reflection
Conveyor belt
Atomic Layer DepositionMetal Roll-to-RollDoor mounted
© 2019 J.A. Woollam jawoollam.com 15
Common In Situ Considerations
Nominal Angle of Incidence
–Determined during „System Check‟ calibration
Window Effects
Substrate Temperature
Substrate Wobble
© 2019 J.A. Woollam jawoollam.com 16
Viewport Window Effects (Strain) SE polarization measurements are not affected
by transparent coatings on chamber windows.
– Beam transmits through window at/near normal incidence.
– Absorbing coatings can decrease signal-to-noise or
eventually limit spectral range if coatings become opaque.
Calibration is required for window birefringence,
which changes the polarization.
– Patented 2nd order window correction applied.
Calibration Data, Channel #10 (3342 Å)
Polarizer Azimuth in degrees
60 80 100 120 140 160 180
Fourier
Coeffic
ients
-0.6
-0.3
-0.0
0.3
0.6
0.9
1.2
AlphaBetaResidualFit
No Window
Correction
Calibration Data, Channel #10 (3342 Å)
Polarizer Azimuth in degrees
60 80 100 120 140 160 180
Fourier
Coeffic
ients
-0.6
-0.3
-0.0
0.3
0.6
0.9
1.2
AlphaBetaResidualFit
Patented 2nd Order
Window Correction
RCE Data Fits, Native Oxide on Si, with Windows
Photon Energy (eV)
0.0 1.0 2.0 3.0 4.0 5.0 6.0 7.0
in d
egre
es
100
120
140
160
180
Model Fit Exp. Data with offset correction applied'raw' Exp. Data
Mount windows / viewports
evenly to minimize induced
window mounting strain
© 2019 J.A. Woollam jawoollam.com 17
Substrate Temperature
Variable Temperature Silicon Optical Constants
Substrate commonly not at room temperature.
Optical constants are temperature dependent.
Temperature and composition dependent material files
available or can be created within the software.
© 2019 J.A. Woollam jawoollam.com 18
Beam Wobble During Substrate Rotation Substrate rotation may cause
beam “wobble”.
– Minimize rotator wobble if possible.
– Use large beam diameter to always
cover receiver (detector) aperture.
– Synchronize data acquisition period
with substrate rotation period.
Or Trigger measurements for specific
position.
Ellipsometer
beam
rotation
Beam
Trajectoryaxis of
rotationq
Beam trajectory due
to Substrate rotation
Detector
aperture
Ellipsometer
beam
© 2019 J.A. Woollam jawoollam.com 19
Synchronization with Rotation Period Beam wobble from rotating substrates can
produce beat pattern in dynamic data when
acquisition period does not match substrate
rotation period.
Right figures show dynamic data initially out
of sync with substrate rotation period.
Data acquisition time changed after 2 minutes
to match substrate rotation period.
Experimental Data
Time in Minutes
60 62 64 66 68 70
Delta
in d
egre
es
99.0
99.5
100.0
100.5
101.0
101.5
102.0
Exp 2.1024eV
© 2019 J.A. Woollam jawoollam.com 20
Growth Example: ALD WO3
Data courtesy
of Veeco/CNT
© 2019 J.A. Woollam jawoollam.com 21
Fast Process Development & Optimization
0 50 100 150 200 250 3000
4
8
12
16
20
F
ilm t
hic
kn
ess (
nm
)
Number of cycles
15 s
60 s
15 s
30 s
0 20 40 60 80 100 120 1400.00
0.02
0.04
0.06
0.08
0.10
Gro
wth
ra
te (
nm
/cycle
)
Plasma exposure time (s)
single deposition run
separate depositions
Monitor film thickness while changing
precursor/reactant dosing time
Calculate growth per cycle from slope
to establish saturation curves
Ex situ measurements not strictly necessary as
single deposition run yields saturation curves, etc.
Slide courtesy of Eindhoven University of Technology
© 2019 J.A. Woollam jawoollam.com 22
Initial Growth: Substrate Dependence, Nucleation Delay
Slide courtesy of Eindhoven University of Technology
0 50 100 150 2000
2
4
6
8
10
TaN on HF-last Si
TiN on SiO2 (1000
oC)
Film
th
ickn
ess (
nm
)
Number of cycles
0 50 100 150 200 250
0
2
4
6
8
10
12 Plasma ALD Pt
Thermal ALD Pt
Th
ickn
ess (
nm
)
Number of cycles
TiN from TiCl4 nucleates poorly on surfaces
with low —OH densities,
TaN from Ta[N(CH3)2]5 nucleates easily
Very long nucleation delay of Pt by
thermal ALD on oxide surfaces,
plasma-assisted ALD nucleates easily
With in situ SE nucleation delay of ALD processes can be investigated
and film thickness can be controlled exactly
© 2019 J.A. Woollam jawoollam.com 23
Distinction of Phase Compositions
Slide courtesy of Eindhoven University of Technology
1 2 3 4 5 60
10
20
30
Die
lectr
ic f
un
ctio
n
2
Photon energy (eV)
Different TaNx phases deposited by varying ALD conditions
Clear distinction TaNx phases from dielectric function:
• Conductive TaN shows Drude absorption by free electrons
• Semiconductive Ta3N5 shows Tauc bandgap behavior
TaN0.45 (390 µ cm)
TaN0.49 (1.0×103 µ cm)
TaN1 (1.1×104 µ cm)
Ta3N4.7
Ta3N5
Langereis et al., J. Appl. Phys. 102, 083517 (2007)
© 2019 J.A. Woollam jawoollam.com 24
Evolving Film Properties: ALD TiN
© 2019 J.A. Woollam jawoollam.com 25
Summary
Spectroscopic Ellipsometry is a useful technique for
monitoring in situ dynamic processes.
– Determine thickness, growth/etch rate, optical constants…
Determine other material properties such as
composition, resistivity, and crystallinity from
optical property changes.
Spectroscopic ellipsometers have been integrated
on a variety of in situ and in-line systems.
THANK YOU!