Oxidation Effects on the Optical Constants of Heavy Metals in the Extreme Ultraviolet Amy Grigg R. Steven Turley Brigham Young University 1 Why Extreme Ultraviolet? Thin Film or Multilayer Mirrors Soft X-Ray Microscope EUV Lithography Earth’s Magnetosphere in the EUV 2 Oxidation Problem High absorption requires thin films. The surfaces of many materials oxidize. At optical wavelengths, this oxidation is often negligible. It is a major issue for our thin films, however. 3 X-Ray Photoelectron Spectroscopy 4 How XPS works K max hv 5 Electron Binding Energy 4500 Th 4000 4f5/2 3500 4f7/2 Counts 3000 2500 2000 Th 4d3/2 4d5/2 O 1s 1500 C 1000 1s 500 0 1000 800 600 400 Th 5d3/2 5d5/2 200 0 Binding Energy (eV) 6 Peak Shifts 3.6K 3.4K 3.2K 3K 2.8K 2.6K 2.4K 2.2K 2K 1.8K 1.6K 1.4K 1.2K 1K 800 600 400 200 354.9 352.9 350.9 348.9 346.9 344.9 342.9 340.9 338.9 336.9 334.9 332.9 330.9 328.9 Thorium peaks on surface 326.9 3.2K 3K 2.8K 2.6K 2.4K 2.2K 2K 1.8K Thorium peaks after oxygen is gone 1.6K 1.4K 1.2K 1K 800 600 400 200 354.9 352.9 350.9 348.9 346.9 344.9 342.9 340.9 338.9 336.9 334.9 332.9 330.9 328.9 326.9 7 Depth Profiling: Method 1 Sputtering: Argon ions knock off individual atoms and drill a hole through the sample 8 Depth Profiling: Method 2 Variable angle scans: Depth is obtained as the analyzer is moved towards incidence θ eee- Sample 9 Variable Angle Results Only penetrates about 80 Angstroms into the sample This allows us to see surface contamination, but not composition with depth Results are averaged: cannot obtain resolved composition with depth 10 Sputtering Results 11 Results This isn’t the true interface because the probability of electron escape is exponential with depth Ideal interface: 12 Results Si interface is not ideal This is likely due to the sputtering process Implantation Sputtering roughness Shape of sputtered area 13 Too Much Oxidation These samples were only a few hours old. We need more uniformity for singlelayer reflectors. Solution: Make ThO2 mirrors. Reflection is also high in EUV and it should be more uniform. 14 ThO2 Results 15 ThO2 Conclusions Fully oxidized thorium is much more uniform. ThO2 shows definite promise as a single-layer reflector in the EUV. 16 Ultimate Goal Determine the optical constants of our materials Ν n ik 1 i 17 Fitting Reflection/Transmission Others have taken the oxide layer into account, but have assumed an ideal interface Measured oxidation (XPS) shows that our approximation is inaccurate 18 Put the Data to Use Incorporate what we know about oxidation into the way we determine our optical constants. Write a data-fitting program Inputs: measured oxidation, reflection/transmission data Outputs: optical constants of measured element (δ and β) 19 Data-Fitting Program Task: Find the most likely optical constants (δ and β) to have produced the measured data that is input Least squares routine: Minimize N ( f ( xi ; , ) yi ) 2 2 i 1 20 Function f ( xi ; , ) Function f uses Matrix Method with Fresnel coefficients to determine theoretical reflection and transmission D1 D2 B U1 U 2 21 Fit and Data 22 23 Continued Research Make a sample, measure it with XPS, model the oxide layer with the program based on the XPS results, and test method Make user interface for program if method works well Determine cause of non-ideal Si interface 24 Acknowledgements A special thanks to R. Steven Turley David Allred Matt Linford BYU Thin Films Group Physics & Astronomy Department Funding ORCA Mentoring Grant NASA Space Grant Images from www.schott.com/magazine/english/info99/ and www.lbl.gov/Science-Articles/Archive/xray-inside-cells.html. 25 Other Results of Interest There was an increase in oxygen when the sample sat for more than 4 or 5 minutes in between sputtering/scans. This was observed for 5 out of 5 samples that sat still between scans. 26 * * * * * indicates where the sample stood for more than 4 or 5 minutes in between scans 27 What Could This Be? Hypothesis: This is likely due to preferential sputtering. The argon ions will knock off oxygen atoms more readily than thorium. While sputtering, scans would show less O than actually exists. 28 Future Research Test preferential sputtering hypothesis. Investigate other peak anomalies: N, Ar 29