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Comparison of heavy ion-induced K-alpha x-ray satellite spectra from gases and solids. [32. 4-MeV O ions]

Technical Report ·
OSTI ID:6672651
A study of the effects of chemical environment on the K-alpha satellite spectra of Si, SiF/sub 4/, SiH/sub 4/, P/sub 4/, S/sub 8/, SF/sub 6/, SO/sub 2/, H/sub 2/S, NaCl, KCl (Cl), CCl/sub 4/, Cl/sub 2/, HCl, Ar and KCl (K) excited by 32.4-MeV oxygen ions has been performed. The average degree of L-shell ionization at the time of K-alpha x-ray emission (as reflected by the satellite relative intensities) is much higher for the light gases SiH/sub 4/, H/sub 2/S, and HCl than for the corresponding heavy gases, solids, and liquid. It was determined from their correlation with local valence electron density that the L-shell ionization states do not depend upon physical state but upon the availability of electrons from neighboring atoms. For atoms with electron-rich ligands, interatomic electron transfer dominates the fast rearrangement occurring prior to K-alpha x-ray emission. The comparison of K-alpha satellite energy shifts with the results of Hartree-Fock calculations provided further support for the above conclusions. A theoretical prediction of multiple ionization employing the binary encounter approximation was found to overestimate the observed degree of L-shell ionization, but considerably improved agreement was obtained by accounting for the increases in L-shell binding energy as L-shell electrons are removed.
Research Organization:
Air Force Inst. of Tech., Wright-Patterson AFB, OH (USA)
OSTI ID:
6672651
Report Number(s):
AD-A-050006; AFIT-CI-78-31
Country of Publication:
United States
Language:
English

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