Satellite structure in the photoelectron spectra of rare gases, some simple gaseous molecules, and alkali metal halides
Description
The rare gases Ar, Kr, and Xe, the alkali metal ions, and several simple molecules were studied to get insight into the excitation mechanism involved in the transitions to excited states. The satellite lines in the photoelectron spectra of both the inner and outer shells were studied. The satellite lines in the photoelectron spectra of the outer shells of the rare gases are compared with optical data. In the case of Ar and Kr, configuration interaction was found to be more important than electron shakeup. The photoelectron spectra of the valence shells of the alkali halides NaCl, KCl, KBr, RbCl and CsCl were run and the satellite structures compared with those of the rare gases. The satellite lines in the spectra of NO, N2O, H2O and N2 are discussed. 9 tables, 24 figures, 66 references
Availability note (English)
MF available from INIS under the Report Number; Available from NTIS.
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Additional details
Publishing Information
- Imprint Pagination
- 103 p.
- Report number
- TID--26944
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 7253241
- Subject category
- S74: ATOMIC AND MOLECULAR PHYSICS;
- Descriptors DEI
- ARGON; CESIUM CHLORIDES; CONFIGURATION INTERACTION; EXCITED STATES; HARTREE-FOCK METHOD; KRYPTON; NITROGEN; NITROGEN OXIDES; PHOTOELECTRON SPECTROSCOPY; POTASSIUM BROMIDES; POTASSIUM CHLORIDES; RUBIDIUM CHLORIDES; SELF-CONSISTENT FIELD; SODIUM CHLORIDES; SUDDEN APPROXIMATION; WATER; XENON
- Descriptors DEC
- ALKALI METAL COMPOUNDS; BROMIDES; BROMINE COMPOUNDS; CESIUM COMPOUNDS; CHALCOGENIDES; CHLORIDES; CHLORINE COMPOUNDS; ELECTRON SPECTROSCOPY; ELEMENTS; ENERGY LEVELS; HALIDES; HALOGEN COMPOUNDS; HYDROGEN COMPOUNDS; NITROGEN COMPOUNDS; NONMETALS; OXIDES; OXYGEN COMPOUNDS; POTASSIUM COMPOUNDS; RARE GASES; RUBIDIUM COMPOUNDS; SODIUM COMPOUNDS; SPECTROSCOPY
Optional Information
- Notes
- Thesis. Available from NTIS. $5.50.