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A Monte Carlo method is used to simulate the vacancy cascade of Xe atom following inner-shell ionization. The calculations have been made by tracing successive radiative and Auger transitions. The effect of electron shakeoff is taken into account. The calculated charge distributions of ions are in good agreement with the experimental results following internal conversion of 131m Xe and X-ray photoionization of Xe gas.
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Takeshi Mukoyama (1986) studied this question.
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