Vacancy Cascades Following Inner-shell Ionization in Ar And Kr Determined Using Different Atomic Data
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概要
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The charge state distribution of ions following K-shell ionization in Ar and Kr atoms is calculated using a Monte Carlo simulation technique. A computer program is written to trace successive X-ray and Auger transition probabilities, which fill vacancies in atomic configurations. The radiative and nonradiative branching ratios are evaluated. Electron shake-off probabilities due to atomic rearrangement after inner-shell ionization are considered in the calculation. The obtained results are compared with those determined experimentally and those calculated from the atomic data collected from different literature sources. It is found that using accurate atomic data leads to results that agree well with experimental values.
- Published by the Japan Society of Applied Physics through the Institute of Pure and Applied Physicsの論文
- 2004-05-15
著者
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El-shemi Adel
Applied Sciences Department College Of Technological Studies
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El-Shemi Adel
Applied Sciences Department, College of Technological Studies, P.O. Box 42325, Shuwaikh 70654, Kuwait