Ion-charge state distributions during vacancy cascades following K - and L I -shell ionization are calculated using a Monte Carlo simulation. The probability P ( n ) that n electrons are ejected after primary ionization is given as a function of atomic number in the region Z = 7 to Z = 60. The calculations are accomplished by tracing successive radiative and non-radiative transitions and the electron shake off process as an additional effect. Radiative and non-radiative transition rates have been calculated as relativistic wave functions.
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El-shemi et al. (1997) studied this question.
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