Thorium Based Thin Films as EUV Reflectors Jed Johnson Honors Defense

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Thorium Based Thin Films as

EUV Reflectors

Jed Johnson

Honors Defense

Reflectors in EUV range

EUV range is about

1001000Å

General Challenges:

- hydrocarbon buildup

- absorption

- high vacuum needed

Complex index of refraction: ñ=n+ik

Applications of EUV Radiation

EUV Lithography Thin Film or Multilayer Mirrors

EUV Astronomy

Soft X-ray Microscopes

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.

Creating Thin Films

• Ions from an induced argon plasma bombard a target. Atoms are then ejected from the target and accumulate as a coating on the substrate.

Measuring Reflectance

Data is taken primarily at the ALS (Advanced Light Source) at

LBNL in Berkeley, CA. Accelerating electrons produce high intensity synchrotron radiation.

Why Actinides?

Beta vs. delta scatter plot at 4.48 nm

Note: Nickel and its neighboring 3d elements are the nearest to uranium in this area.

ñ r

 n

 ik

1

   i

 

1

 n ,

  k

Periodic table

δ vs. (δ + β)

30.4 nm (41 eV)

Thorium vs. Uranium

Why such a large difference in optical properties?

Thorium (11.7 g/cm^3) is less dense than uranium

(19.1 g/cm^3).

0.7

0.6

0.5

0.4

0.3

1

0.9

0.8

0.2

0.1

0

0

Calculated Reflectance vs. energy (eV) at 5 deg

100 200 300

Photon Energy

400 500

Gold

Ir

Ni

U

Thorium

However….

The mirror’s surface will be oxidized.

At optical wavelengths, this oxidation is negligible. It is a major issue for our thin films though.

Problems with Uranium

Immediate oxidation to UO

2

. (10 nm in 5 min)

Further oxidation to U

2

O nm in six to 12 months)

5 is less rapid. (5 – 10

Can even proceed to UO

3

!

Lower density = lower reflectance

A Possible Alternative: Thorium

Only one oxidation state:

ThO

2

. We know what we have!

The densities of UO

2

11 g/cm 3 ) and ThO

2 g/cm 3 ) are similar.

(about

(9.85

Rock stable: Highest melting point (3300 deg C) of any known oxide.

0.9

0.8

0.7

0.6

0.5

0.4

0.3

0.2

0.1

0

0

Calculated Reflectance vs. energy (eV) at 10 deg

Reflectance, S polarization at 10 degrees of various materials

100 200

Au

300

Energy in eV

Ni ThO2

400

UO2

500 600

0.2

0.1

0

0

0.6

0.5

0.4

0.3

0.7

0.8

First Thorium Reflectance Data

(Nov. ‘03 ALS)

M e asure d Re fle ctance of Th02 at 10 de gre e s

5

2.16-2.8 nm

12.4-18.8 nm

10

2.7-4.8 nm

17.2-25.0

15 20

Wavelength (nm)

4.4-6.8 nm

22.5-32.5

6.6-8.8 nm

25

8.4-11.6 nm

30

11.0-14.0 nm

35

Th vs. EUV Other Reflectors

0.9

0.8

0.7

0.6

0.5

0.4

0.3

0.2

0.1

0

2

Th001

UO2

UN

NiO on Ni

Ir

Au

4 6

Wavelength (nm)

8 10 12

Between 6.5 and 9.4 nm, Th is the best reflector we have measured.

Measured and Calculated

Reflectance at 10 deg

0.9

0.8

0.7

0.6

0.5

0.4

0.3

0.2

0.1

0

0 5

2.16-2.8 nm

8.4-11.6 nm

22.5-32.5

10 15 20

Wavelength (nm)

25

2.7-4.8 nm

11.0-14.0 nm calc. AFM CXRO S polarized

4.4-6.8 nm

12.4-18.8 nm

30

6.6-8.8 nm

17.2-25.0

35 40

1.00

0.90

0.80

0.70

0.60

0.50

0.40

0.30

0.20

0.10

0.00

70 80

“Zoomed in”

(and nm  eV) calc ThO2 42nm

Th001 measured

Th001 measured

Th001 measured

Th001 measured

90

Energy (eV)

100 110 120

1.00

0.90

0.80

0.70

0.60

0.50

0.40

0.30

0.20

0.10

0.00

100

Higher Energies calc ThO2 42nm

Th001 measured

Th001 measured

Th001 measured

Th001 measured

Th001 measured

Th001 measured

150 200

Energy eV

250 300

Einstein’s Atomic Scattering Factor

Model

Photons are scattered principally off electrons.

More electrons = higher reflection.

Assumption: condensed matter may be modeled as a collection of noninteracting atoms. In the higher energy EUV, chemical bonds shouldn’t contribute. (except near threshold regions)

Can the ASF model be applied in the visible light range?

Silicon (opaque) and oxygen

(colorless gas) combine to form

SiO

2

(quartz).

Clearly the chemical bonds have a dramatic effect on the compound’s properties.

Where then is the ASF model valid?

At some point,

ASF model and measured data should converge.

Unpublished

BYU study: SiO

2 plots never converged up to

300 eV.

Possibility #1

Bad experiment! Data has never been so clean though and the features are clear. Curve was reproduced March

2004.

Beamline 6.3.2 coordinator at ALS has no explanation.

M e asure d Re fle ctance of Th02 at 10 de gre e s

0.8

0.7

0.6

0.5

0.4

0.3

0.2

0.1

0

0 5

2.16-2.8 nm

12.4-18.8 nm

10

2.7-4.8 nm

17.2-25.0

15 20

Wavelength (nm)

4.4-6.8 nm

22.5-32.5

6.6-8.8 nm

25

8.4-11.6 nm

30

11.0-14.0 nm

35

Possibility #2

The sputtered film wasn’t pure thorium.

Possibly an alloy?

EDX w/ SEM indicates 

Carbon and Oxygen

Cutting fluid residue left on target?

Thorium carbide?

Hydrocarbon contaminant?

Carbon Impurities in silicon? (EDX “sees through”)

Surface XPS only sees Th.

Bottom Line: none of these small contributions could have caused a drop from ~70% to ~10% reflectance.

Possibility #3

Maybe chemistry IS playing a larger role in this region than previously expected.

Could the atomic scattering model need modification in this range?

Transmission Measurements

Below 14 nm, there is a feature common to reflection and transmission measurements.

1

0.9

0.8

0.7

0.6

0.5

0.4

0.3

0.2

0.1

0

12 13 14

Reflection at 10 deg

Transmission at near-normal incidence

15 wavelength (nm)

16 17 18

Optical Constant Fitting

Th003 is the only transmission sample to be made and analyzed to date.

Least squares procedure fits for optical constants and film thickness.

Characterization Issues

Film thickness

(more XRD and ellipsometry)

Film composition

(XPS)

Roughness (AFM)

Optical Constant Data

17.0 nm 13.9 nm

Comparison: Calculated beta from transmission.

17.0 nm: 0.0330 13.9 nm: 0.1078 thickness: 197 Ǻ (XRD)

Good Agreement!

Conclusions

1. Th exhibits the highest reflectance of any measured compound from 6.5 to 9.4 Ǻ.

2. The Atomic Scattering Factor model may need revision in the EUV.

3. Constants obtained from the fitting program are reasonable.

Future Research

Film oxidation (rate)

Film composition (modeling grain boundaries, interfaces)

ThO

2 constant determination

Roughness effects on reflectance / modeling

Theoretical ASF research

Acknowledgments

BYU XUV Research Group colleagues

Dr. David D. Allred

Dr. R. Steven Turley

BYU Physics Department Research

Funding

X-Ray Absorption Near Edge

Structure (XANES)

Induced current is measured in wire connected to sample as EUV photons strike it.

Absorption information.

Theoretical multiple scattering calculations are compared with experimental XANES spectra in order to determine the geometrical arrangement of the atoms surrounding the absorbing atom.

XANES Data

5

4.5

4

3.5

3

2.5

2

1.5

1

0.5

0

66

Th004(Si)

ThO2(Si)

UO14g(Si)

UO12g(Si)

71 76 81

Energy (eV)

86 91 96

More XANES Data

Relative Intensity

3

2.5

2

1.5

1

0.5

0

270

ThO2

UO12g

Th004

275 280 285 290

Energy (eV)

295 300 305 310

XANES and Beta

0.14

0.12

0.1

0.08

0.06

0.04

0.02

0

12 13 beta

XANES Th004

XANES ThO2

14 15 wavelength (nm)

16 17 18

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