giovanni terenziani hipims development for superconducting cavities
TRANSCRIPT
Development of HIPIMS Technology for
Superconducting Coated Cavities
G. Terenziani, S.Calatroni, A. P. Ehiasarian, T. Junginger, S. Aull
Outline
• From Dc Magnetron Sputtering to HiPIMS
• HIPIMS Samples Analysis:
OES
MS
SEM
XRD
RRR
• HIPIMS Cavity Results
From DCMS To HiPIMS
© Andre Anders, 201011
Generalized Structure Zone Diagram
A. Anders, Thin Solid Films 518, 4087 (2010).
derived from Thornton’s diagram, 1974
Based on “Structure Zone Model” - Thornton, J.Vac. Sci. Technol. 11 (1974) 666
Outline
• From Dc Magnetron Sputtering to HiPIMS
• HIPIMS Samples Analysis:
OES
MS
SEM
XRD
RRR
• HIPIMS Cavity Results
Vacuum, Surfaces & Coatings Group
Technology Department
HIPIMS Samples – Optical Emission
Spectroscopy (OES)
50 88 125 165 180 270 340 410 480 550
21
37
53
69
85
Pulse Duration (µs)
Peak
Curr
ent
(A)
0.05000
0.1250
0.2000
0.2750
0.3500
0.4250
0.5000
0.5750
0.6500
Nb II / Nb I Ratio
G. Terenziani, S. Calatroni, A.P. Ehisarian, T.
Junginger12
Vacuum, Surfaces & Coatings Group
Technology Department
HIPIMS Samples – Optical Emission
Spectroscopy (OES)
0
0.02
0.04
0.06
0.08
0.1
0.12
0.14
0.16
0.18
0 0.2 0.4 0.6 0.8 1 1.2
Ra
tio
Nb
+/N
b
Current Density (A*cm-2)
Ratios (Nb+/Nb) vs Peak Current Density @ different pulse width
Ratio I @ 50 us
Ratio I @ 200 us
Ratio I @ 550 us
G. Terenziani, S. Calatroni, A.P. Ehisarian, T.
Junginger13
Outline
• From Dc Magnetron Sputtering to HiPIMS
• HIPIMS Samples Analysis:
OES
MS
SEM
XRD
RRR
• HIPIMS Cavity Results
Vacuum, Surfaces & Coatings Group
Technology Department
0 20
1
10
100
1000
10000
100000
1000000
Inte
nsity
Energy
Equation y = a + b*x
Weight No Weighting
Residual Sum of Squares
0.03801
Pearson's r -0.99042
Adj. R-Squar 0.98028
Value Standard Erro
IntensityIntercept 5.44624 0.02626
Slope -0.2808 0.00727
0 20
1
10
100
1000
10000
100000
1000000
Inte
nsity
Energy
Equation y = a + b*x
Weight No Weighting
Residual Sum of Squares
0.37334
Pearson's r -0.99248
Adj. R-Square 0.98487
Value Standard Erro
IntensityIntercept 4.86924 0.02183
Slope -0.16911 0.0021
0 20
1
10
100
1000
10000
100000
1000000
Inte
nsity
Energy
Equation y = a + b*x
Weight No Weighting
Residual Sum of Squares
0.03287
Pearson's r -0.99008
Adj. R-Square 0.97922
Value Standard Error
IntensityIntercept 5.87232 0.01752
Slope -0.46038 0.01499
Zone I Zone II
Zone III
HIPIMS Samples – Mass Spectrometer
(MS) – Nb+
case – 0.5 Acm-2
59.5% 29%
11%
G. Terenziani, S. Calatroni, A.P. Ehisarian, T.
Junginger15
Vacuum, Surfaces & Coatings Group
Technology Department
0 20
1
10
100
1000
10000
100000
1000000
Inte
nsity
EnergyeV
Equation y = a + b*x
Weight No Weighting
Residual Sum of Squares
0.01586
Pearson's r -0.98183
Adj. R-Squar 0.96
Value Standard Erro
IntensityIntercept 5.97114 0.02368
Slope -0.6212 0.04002
0 20
1
10
100
1000
10000
100000
1000000
Inte
nsity
EnergyeV
Equation y = a + b*x
Weight No Weighting
Residual Sum of Squares
0.01039
Pearson's r -0.99757
Adj. R-Square 0.99498
Value Standard Error
IntensityIntercept 5.68381 0.01009
Slope -0.29305 0.0038
0 20
1
10
100
1000
10000
100000
1000000
Inte
nsity
EnergyeV
Equation y = a + b*x
Weight No Weighting
Residual Sum of Squares
0.17679
Pearson's r -0.99539
Adj. R-Squar 0.99071
Value Standard Erro
IntensityIntercept 5.08897 0.01364
Slope -0.1489 0.00144
Zone I Zone II
Zone III
HIPIMS Samples – Mass Spectrometer
(MS) – Nb+
case – 1.3 Acm-2
49.5% 33.3%
12%
G. Terenziani, S. Calatroni, A.P. Ehisarian, T.
Junginger16
Vacuum, Surfaces & Coatings Group
Technology Department
0 5 10 15 20 25 30
1
10
100
1000
10000
100000
1000000
Inte
nsity
Energy
Equation y = a + b*x
Weight No Weighting
Residual Sum of Squares
0.01735
Pearson's r -0.98468
Adj. R-Square 0.96621
Value Standard Error
IntensityIntercept 6.01073 0.02477
Slope -0.70913 0.04186
0 10 20 30
1
10
100
1000
10000
100000
1000000
Inte
nsity
Energy
Equation y = a + b*x
Weight No Weighting
Residual Sum of Squares
0.26334
Pearson's r -0.99737
Adj. R-Square 0.99471
Value Standard Error
IntensityIntercept 5.37594 0.00808
Slope -0.14611 9.00585E-4
0 20
1
10
100
1000
10000
100000
1000000
Inte
nsity
Energy
Equation y = a + b*x
Weight No Weighting
Residual Sum of Squares
1.65281
Pearson's r -0.97238
Adj. R-Square 0.94526
Value Standard Error
IntensityIntercept 4.16017 0.02843
Slope -0.06511 0.00111
Zone I Zone II
Zone III
HIPIMS Samples – Mass Spectrometer
(MS) – Nb+
case – 2 Acm-2
48.4%
50.6%
1%
G. Terenziani, S. Calatroni, A.P. Ehisarian, T.
Junginger17
Outline
• From Dc Magnetron Sputtering to HiPIMS
• HIPIMS Samples Analysis:
OES
MS
SEM
XRD
RRR
• HIPIMS Cavity Results
Vacuum, Surfaces & Coatings Group
Technology Department
DCMS Cross Section Structure
G. Terenziani, S. Calatroni, A.P. Ehisarian, T.
Junginger22
1 um
Cu
Nb
C
Surface features in HIPIMS seem larger
than in DCMS but the column size in
cross section appears smaller in
HIPIMS. The large surface features in
HIPIMS could be comprised of several
columns whose inter-columnar
boundaries are so dense that they
appear as single crystals.
Vacuum, Surfaces & Coatings Group
Technology DepartmentG. Terenziani, S. Calatroni, A.P. Ehisarian, T.
Junginger23
Cross Section Structure -
Comparison
In neither DCMS nor HIPIMS there doesn't seem to be a large-scale epitaxial growth of
the films. Rather, the growth in both cases starts out with numerous nucleation sites
probably with different grain orientation and the subsequent growth is a competition
between different grain orientations.
In HIPIMS it seems that near the coating-substrate interface there is a thicker region
where there is competitive growth.
This is followed by a process of grain selection where winning grains widen to take up
the entire area.
It could be speculated that during the selection process, DCMS grains do not densify
their grain boundaries whilst HIPIMS grains can do that due to the extra surface mobility
of metal ions.
Because of this the morphology of the HIPIMS surface appears to contain larger
features than DCMS.
Outline
• From Dc Magnetron Sputtering to HiPIMS
• HIPIMS Samples Analysis:
OES
MS
SEM
XRD
RRR
• HIPIMS Cavity Results
Vacuum, Surfaces & Coatings Group
Technology Department
HIPIMS Samples – X-Ray Diffraction
Cu <200>
Cu <200>
Cu <200>
Nb <110>
Nb <110>
Nb <110>
G. Terenziani, S. Calatroni, A.P. Ehisarian, T.
Junginger25
Vacuum, Surfaces & Coatings Group
Technology Department
HIPIMS Samples – X-Ray Diffraction
G. Terenziani, S. Calatroni, A.P. Ehisarian, T.
Junginger26
0
1
2
3
4
5
6
0
5
10
15
20
25
0 0.5 1 1.5 2 2.5
Thic
kne
ss (
um
)
Rat
io N
b<1
10
> /
Cu
<2
00
>
Current Density (A/cm2)
Ratio
Sample Thickness
Outline
• From Dc Magnetron Sputtering to HiPIMS
• HIPIMS Samples Analysis:
OES
MS
SEM
XRD
RRR
• HIPIMS Cavity Results
Vacuum, Surfaces & Coatings Group
Technology Department
HIPIMS Samples – Residual
Resistance Ratio (RRR)
G. Terenziani, S. Calatroni, A.P. Ehisarian, T.
Junginger28
0
5
10
15
20
25
0
5
10
15
20
25
0 0.5 1 1.5 2 2.5 3
Nb
<11
0> / C
u <2
00
>
RR
R
Current Density (A/cm2)
Comparison RRR Vs Crcistallographic Orientation
RRR Vs Current Density @200 us
Nb <110> / Cu <200>
Outline
• From Dc Magnetron Sputtering to HiPIMS
• HIPIMS Samples Analysis:
OES
MS
SEM
XRD
RRR
• HIPIMS Cavity Results
Vacuum, Surfaces & Coatings Group
Technology Department
HIPIMS on 1.3 GHz Cavity – Deposition System
1.3 GHz Cavity
Magnet
Central Cathode
413 mm
G. Terenziani, S. Calatroni, A.P. Ehisarian, T.
Junginger30
Vacuum, Surfaces & Coatings Group
Technology Department
HIPIMS on 1.3 GHz Cavity M2.3 – Rs
Vs T
Δ/kb = 18 K
RRR = 13.1
RRES = 4.5 nΩ
G. Terenziani, S. Calatroni, A.P. Ehisarian, T.
Junginger31
J = 2 A/cm2, τ = 200 us
Surface treatment: EP + SUBU
Vacuum, Surfaces & Coatings Group
Technology Department
HIPIMS on 1.3 GHz Cavity M2.7 – Rs
Vs T
Δ/kb = 18 K
RRR = 15
RRES = 6.5 nΩ
G. Terenziani, S. Calatroni, A.P. Ehisarian, T.
Junginger32
J = 2 A/cm2, τ = 200 us
Surface treatment: EP
Vacuum, Surfaces & Coatings Group
Technology DepartmentG. Terenziani, S. Calatroni, A.P. Ehisarian, T.
Junginger33
There is an increase of
about 15 nΩ from low field
to 15 MV/m between the
curves measured just
below and just above λ
transition
Q-slope is influenced by
thermal boundary, but it is
not the dominant effect
(≈7%)
HIPIMS on 1.3 GHz Cavity M2.7 – Rs
Vs
Eacc
Vacuum, Surfaces & Coatings Group
Technology Department
HIPIMS on 1.3 GHz Cavity - Results
G. Terenziani, S. Calatroni, A.P. Ehisarian, T.
Junginger34