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Ion-excited K. cap alpha. x-ray satellite spectra of Si, S, Cl, and Ar in the gas phase

Journal Article · · Phys. Rev., A; (United States)
The K..cap alpha.. satellite spectra of Si in the gases SiH/sub 4/ and SiF/sub 4/, of S in the gases H/sub 2/S, SO/sub 2/, and SF/sub 6/, of Cl in the gases HCl and Cl/sub 2/ and in the liquid CCl/sub 4/, and of gaseous Ar produced by bombardment with oxygen ions were examined in detail and compared with the spectra of solid compounds obtained in a previous study. It was found that the apparent average state of L-shell ionization at the time of K..cap alpha.. x-ray emission does not depend upon the physical state, but upon the availability of electrons from nearest-neighbor atoms. The K..cap alpha.. satellite energies in conjunction with Hartree-Fock calculations provide a measure of the average numbers of missing M-shell electrons, and this information further supports the conclusion that interatomic electron transfer dominates the fast rearrangement occurring prior to K..cap alpha.. x-ray emission in atoms having highly depleted M shells. Various K..cap alpha.. satellite peak-broadening mechanisms were considered and it was found that broadening due to the distribution of M-shell vacancies accounts for a significant portion of the total peak width.
Research Organization:
Cyclotron Institute and Department of Chemistry, Texas AandM University, College Station, Texas 77843
OSTI ID:
6842743
Journal Information:
Phys. Rev., A; (United States), Journal Name: Phys. Rev., A; (United States) Vol. 17:4; ISSN PLRAA
Country of Publication:
United States
Language:
English