Abstract

The photoionisation cross sections for 3d10 subshells are calculated for the elements of the isoelectronic series of atomic Xe such as I-, Xe, Cs+, Ba2+ and La3+. The non-relativistic random-phase approximation with exchange (RPAE) is used to account for the static rearrangement. The maxima in Xe and I- spectra are due to the 3d- epsilon f transition into the continuum, and those for Ba2+ and La3+ are due to 3d-4f transitions to discrete levels. The photoabsorption cross section for Cs+ appears to be sensitive to the method of calculation; RPAE leads to maxima in the discrete spectrum, whereas the static rearrangement leads to a maximum in the continuum. Allowance for the rearrangement due to a 3d-vacancy decay lowers the cross section in the continuum, shifting the oscillator strengths to the discrete spectrum which reveals the existence of the so-called 'collapse' of the 4f electron.

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