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Published January 28, 2024 | Version Published
Journal Article Open

A critical review and meta-analysis of xenon-on-carbon sputter yield data

Creators

  • Polk, James E.1
  • 1. ROR icon California Institute of Technology

Abstract

A systematic review and meta-analysis of sputter yield data for xenon ions normally incident on graphite at energies below 2000 eV was undertaken to identify systematic errors, determine the best model parameter values to represent yield as a function of energy, quantify uncertainty, and determine if the data support differences in yields for different types of graphite. A critical examination of the 11 published data sets for high density graphite, pyrolytic graphite, and amorphous carbon showed that, in general, they were carefully controlled to minimize errors. The most significant quantifiable systematic errors were those caused by the neglect of doubly charged ions, chemical erosion, and the impact of secondary electron emission on ion flux measurements. The effects of gas uptake and outgassing on mass loss measurements and unrepresentative surface textures may have biased other experiments, but these effects could not be quantified. The semi-empirical Eckstein model for yield as a function of energy was fit to data for the three graphite types using a hierarchical Bayesian statistical model, producing recommended fit parameters and probability distributions representing uncertainty in yields. The results showed that differences in yield for high density graphite and pyrolytic graphite were not statistically significant. Apparent differences in yield for amorphous carbon disappeared when the single data set available for energies below 150 eV was corrected for reasonable values of double ion content. Recommended procedures to avoid systematic errors and additional experiments and modeling to fill in gaps in our understanding are included.

Copyright and License

© 2024 Author(s). Published under an exclusive license by AIP Publishing.

Acknowledgement

The research described in this paper was carried out in part at the Jet Propulsion Laboratory, California Institute of Technology, under a contract with the National Aeronautics and Space Administration. The author would like to thank Colleen Marrese-Reading for help collating the data, and John Williams and Seth Thompson at Colorado State University, Russ Doerner at the University of California San Diego, and Daniel Spemann at the Leibniz Institute of Surface Engineering for a number of useful inputs on the experimental methods employed at their respective institutions.

Contributions

James E. Polk: Conceptualization (lead); Data curation (lead); Formal analysis (lead); Funding acquisition (lead); Investigation (lead); Methodology (lead); Project administration (lead); Resources (lead); Software (lead); Validation (lead); Visualization (lead); Writing – original draft (lead); Writing – review & editing (lead).

Data Availability

Data, including parameters for the Stan code to reproduce the fit and samples from the joint posterior distribution, are available from the author upon reasonable request.

Conflict of Interest

The authors have no conflicts to disclose.

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ISSN
1089-7550

Funding

National Aeronautics and Space Administration
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Keywords and subjects

Keywords

  • General Physics and Astronomy

Details

DOI
10.1063/5.0180720
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DOI

10.1063/5.0180720

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Resource type
Journal Article
Publisher
AIP Publishing
Published in
Journal of Applied Physics, 135(4), 040701, ISSN: 0021-8979, 2024.
Languages
English

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  • No commercial reproduction, distribution, display or performance rights in this work are provided.
    No further description.

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Created
January 24, 2024
Modified
January 28, 2025
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