Abstract
The Kα satellite spectra arising from the correlative multielectron processes accompanying K-shell photoionization of Ca, Ti and V were measured using a broad range crystal spectrometer. Multiconfiguration Dirac–Fock calculations were performed to interpret the observed x-ray energies and the spectral line shape. The calculations agree fairly well with the experimental results. The variation of the Kα L1 satellite and the Kα1,2h hypersatellite intensities was measured as a function of excitation energy in the range of 8–35 keV. The Kα L1/Kα1,2 intensity ratio for each element is already saturated in our energy range, and the asymptotic values of 1.58 ± 0.08, 1.26 ± 0.06 and 0.97 ± 0.05 % for Ca, Ti and V were determined. By combining the present results and the previously measured values for various elements, we have found a Z−3.5 scaling law for the Kα L1/Kα1,2 intensity ratio. The measured Kα1,2h/Kα1,2 intensity ratio, for each element, is found to increase smoothly from its onset and shows a long saturation range extending up to at least 25 keV above the threshold for Ti. The evolution of the Kα1,2h/Kα1,2 intensity ratio is compared with the analytic Thomas model and with the theoretical calculation based on the screened hydrogenic model.
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