Abstract
The charge distributions of Xe ions as a result of photoionisation have been studied experimentally and theoretically. The initial vacancies are produced by 4.1-8.0 keV synchrotron orbital radiation and the charge distribution of ions was measured with a time-of-flight mass spectrometer at various photon energies. The theoretical estimation of the charge distribution was made by the use of the Monte Carlo simulation. The calculated charge distributions as a function of incident photon energy are in good agreement with the measured results.
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