Transcript Uranium Oxide as a Highly Reflective Coating

Uranium Oxide and Uranium Nitride as
Highly Reflective Coatings from 2.7 to 11.6
Nanometers
Richard L. Sandberg, Marie K. Urry, Shannon Lunt
David D. Allred, R. Steven Turley
Thanks to
Fellow EUV Members: Jed E. Johnson, Luke J. Bissel, Kristi R. Adamson, Nikki Farnsworth,
William R. Evans, and others from EUV Group, Andy Aguila & Eric Gullickson at ALS/CXRO
Funding: SPIE Scholarship, BYU Physics Dept. Funding, BYU ORCA Scholarship
BYU EUV Optics
April 19, 2004
Why Extreme Ultraviolet (EUV) and Soft X-Rays?
Thin Film or Multilayer Mirrors
EUV Lithography
(making really small computer chips)
EUV Astronomy
Soft X-Ray Microscopes
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The Earth’s magnetosphere in the EUV
Images from www.schott.com/magazine/english/info99/ and www.lbl.gov/Science-Articles/Archive/xray-inside-cells.html.
April 19, 2004
Why Uranium?
•
•
•
•
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Pros: high density and many electrons (92) for absorption, high theoretical
reflectivity: low absorption and high index of refraction
Con: chemically reactive (oxidizes in air to most abundant natural oxide UO2 at STP)
We study different compounds of uranium, such as uranium dioxide (UO2) and
uranium mononitride (UN), in search of compounds with the highest reflectance and
most chemical stability.
Previous Success: IMAGE Satellite Mirror Project—BYU uranium based mirrors
(Launched March 25, 2000)
Delta vs. beta plot for several elements at 4.48 nm
4.48nm
Note: Nickel and its neighboring 3d elements are the
nearest to uranium in this area.
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~  n  ik  1    i
n
r
  1  n,
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 k
Computed Reflectance at 10 degrees of various materials
0.9
0.8
Reflectance
0.7
0.6
0.5
0.4
0.3
0.2
0.1
0
2
4
6
8
Au
10
12
Wavelength (nm)
Ni
UO2
14
U
16
Ir
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Reflectance computed using the CXRO Website: http://www-cxro.lbl.gov/optical_constants/mirror2.html
April 19, 2004
18
20
Sample Preparation
The UO, UN, Ni, and Au samples were deposited
on pieces polished silicon test wafers (100
orientation). Quartz crystal monitors were used to
measure the sputtering and evaporation rates.
•U DC Magnetron/RF Sputtering
The uranium sputter targets used here were of
depleted uranium metal (less than 0.2% U-235).
After sputtering, the uranium oxide was allowed to
oxidize naturally in laboratory air. Uranium
nitride was reactively sputtered (RF) in nitrogen
partial pressure of about 10-5 torr, bellow 10-4 torr
as suggested by L. Black et al., Journal of Alloys
and Compounds 315, 36-41 (2001).
Schematic of DC magnetron
sputtering system at BYU.
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•Ni/Au Resistive Thermal Evaporation
Evaporated Ni wire/Au beads from a resistively
heated tungsten boat (RD Mathis Co.) in a large,
cryopumped, stainless steel “bell jar” coater.
•Ir Sample Prepared at Goddard Space Flight
Center on Glass Slides
Thickness Determined by XRD
Film thickness (nm)
50
y = 40.398x2 - 116.4x + 109.12
R2 = 0.9995
45
40
35
UN (Dens.=14.3)
30
Poly. (UN
(Dens.=14.3))
25
0.6
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April 19, 2004
m λ = 2d sin θ
0.8
1
1.2
Theta (for 4 peaks)
1.4
•XRD Sample Thickness
-UO2
30.0 nm (ρ=10.97 g/cm3)
-UN
38.0 nm (ρ=10. g/cm3)
-NiO on Ni 49.7 nm (ρ=6.67 g/cm3)
-Au
29.5 nm (ρ=19.3 g/cm3)
-Ir
??
(ρ=22.42 g/cm3)
Oxidation of a UN Thin Film
Percent change in thickness
115
110
105
IMD data
Fit
100
95
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10
Time (hrS.)
100
1000
Studying Our Samples
Ellipsometry
Scanning/Transmission Electron
Microscopes (SEM/TEM)
X-ray Photoelectron Spectroscope (XPS)
Atomic Force Microscopy (AFM)
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Images courtesy of www.weizmann.ac.il/surflab/peter/afmworks, www.mos.org/sln/SEM/works/
5
Taking Reflectance Measurements at the ALS
(Advance Light Source)
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• Small Discrepancies arise from
one region to another with the use
of different filters.
•XANES Capability
• Normalization given by
R=(Idetector-Idark)/(Ibeam-Idark)
Reflectance
Beamline 6.3.2 Reflectometer
• Bright synchrotron radiation
• 1-24.8 nm range
• High spectral purity
• Energy/wavelength or θ-2θ
scan capability
Sample of Data from the ALS
0.9
0.8
0.7
0.6
0.5
0.4
0.3
0.2
0.1
0
2.5
Inage courtesy of http://www.lbl.gov/
4.5
6.5
8.5
Wavelength (nm)
10.5
12.5
ALS Measured Reflectance Comparison at 5 deg
0.9
0.8
0.7
Reflectance
0.6
0.5
0.4
UO2
UN
NiO on Ni
Ir
Au
0.3
0.2
0.1
0
2
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3
4
5
6
7
Wavelength (nm)
8
9
10
11
12
ALS Measured Reflectance Comparison at 10 deg
0.7
0.6
UO2
UN
NiO on Ni
Ir
Au
Reflectance
0.5
0.4
0.3
0.2
0.1
0
2
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4
6
8
Wavelength (nm)
10
12
ALS Measured Reflectance Comparison @ 15 deg
0.5
UO2
UN
NiO on Ni
Ir
Au
0.45
0.4
Reflectance
0.35
0.3
0.25
0.2
0.15
0.1
0.05
0
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4
5
6
7
8
Wavelength (nm)
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9
10
11
12
Optical Properties of Uranium Oxide
and Uranium Nitride
n~r  n  ik  1    i
  1  n,
f p ,m
f s ,m
 k
N m21q m  N m2q m 1
 2
N m 1q m  N m2q m 1
qm  qm1

qm  qm1
δ and β of UN from M. Urry
λ (nm)


13
0.01152
0.0595
14
0.0138
0.0416
δ and β of UO2 obtained from S. Lunt’s Thesis
ALS Measured
λ (nm)
q m  N m2  cos 2  i
β
δ
CXRO Calculated
β
δ
4.6
0.0065
8.09E-04
0.0116
0.0011
5.6
0.0103
0.0012
0.0187
0.0025
f p ,m  rp ,m 1
6.8
0.0173
0.004
0.0302
0.0065
1  f p ,m rp ,m 1
8.5
0.0298
0.0151
0.0491
0.0271
10
0.0344
0.0458
0.0674
0.0693
12.5
-0.0038
0.0129
0.0057
0.0399
14
0.0229
0.0103
0.0509
0.017
V.G. Kohn. Phys. Stat. Sol. 185(61), 61-70 (1995).
15.5
0.0362
0.0158
0.0782
0.0281
L.G. Parratt. Physical Review 95 (2), 359-369 (1954).
17.5
0.0547
0.0246
0.1058
0.0464
rs ,m  C m4
f s ,m  rs ,m 1 rp ,m  C
1  f s ,m rs ,m 1
4
m
C m  e iqm Dm / 
Reflectance
Measured Data compared with CXRO Atomic Scattering Factor Model
1
0.9
0.8
0.7
0.6
0.5
0.4
0.3
0.2
0.1
0
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UOx
Comp UO2
Comp UO2 with C cap
2.5
3
3.5
Wavelength (nm)
4
4.5
Photons are scattered
principally off
electrons. More
electrons = higher
reflection.
5
1
0.9
Measured reflectance features
do not agree with CXRO
atomic scattering factors.
More work need to be done
on measuring uranium’s
optical constants.
Reflectance
0.8
0.7
0.6
0.5
0.4
Measured UO2
Computed UO2 (d=30 nm)
Computed UO2 with 0.5 nm C on top
Computed UO2 with C(density=1.5g/cc) 3 nm
0.3
0.2
0.1
0
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April 19, 2004
2.5
4.5
6.5
8.5
Wavelength (nm)
10.5
12.5
XANES (X-Ray Absorption Near Edge Spectroscopy)
XANES at ALS show additional absorption resonances not
accounted for in ASF Data at CXRO.
Relative XANES Scans of UO2 and ThO2
Relative Intensity
1.8
U NVIOIV @ 286.3 eV *
1.6
ThO2
1.4
UO2
1.2
1
0.8
0.6
0.4
280
285
295
290
300
Energy (eV)
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April 19, 2004
*D. R. Lide (ed.), CRC Handbook of Chemistry and Physics,
71st edition, CRC Press, Boca Raton, 1990-91, p.10-256.
305
Conclusions
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Goals
UO2 and UN reflect significantly more •
than Ni, Ir, and Au, the current
materials with highest reflectance,
between 4 and 9 nm.
•
U reflectance differs from the
reflectance predicted by the atomic
scattering factor model (ASF).
Current preparation of UN is not stable
in ambient air (oxidizes to UO2).
Need to test oxidation of heated UN
sample
Determine the optical properties of
UO2 below Shannon’s data (4.5 nm)
and fill out UN optical properties data.
Work with CXRO to amend the
existing uranium atomic scattering
factor data.
Questions?
EUV Group Contact
Dr. David Allred
[email protected]
(801) 422-3489
BYU EUV Optics
April 19, 2004
THANK YOU!!