Abstract
The production of ions with two K vacancies is of fundamental interest in ion-atom collisions1–3. Previously, double K-vacancy production has been inferred from the ratio R = σ hx /σx of hyper-satellite-to-single K-vacancy x-ray yields, assuming the fluorescence yields for single and double K-vacancies are the same1. This ratio has been used to determine double K-vacancy sharing ratios between target and projectile in near symmetric collisions3 and to determine branching ratios for two-electron-one-photon transitions4,5. In these works, it was tacitly assumed that R does not depend upon the target thickness.
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References
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In refs. 6,7 and 9 σOI is denoted by σv, the vacancy production cross section, and σIO is denoted by the sum σc + στ where σc is the cross section for capture to the K shell and στ is the cross section for radiative or Auger decay.
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© 1981 Plenum Press, New York
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Tanis, J.A., Shafroth, S.M., Willis, J.E., Mowat, J.R. (1981). Three-Component Model Analysis of C1 Projectile Hypersatellite K X-Ray Intensities vs C Foil Thickness. In: Fabian, D.J., Kleinpoppen, H., Watson, L.M. (eds) Inner-Shell and X-Ray Physics of Atoms and Solids. Physics of Atoms and Molecules. Springer, Boston, MA. https://doi.org/10.1007/978-1-4615-9236-5_6
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DOI: https://doi.org/10.1007/978-1-4615-9236-5_6
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