Ab initio calculations of branching ratios and cross-sections for inner- and outer-valence levels of SF6 have been carried out by means of the static exchange (STEX) approximation including full intrachannel interaction. The calculations cover an energy region up to 90 eV for the outer and 130 eV for the inner valence molecular levels and the results are compared with experimental data. It is shown that the molecular orbital static exchange method successfully reproduces the strong multiple resonances in the near continuum. The resonances and the energy dependence of the photoionization cross-sections have been used to settle some assignment problems in the valence photoelectron spectrum of SF6. Photoelectron spectra associated with the 2e(g), 3(1u) and 4a(1g) inner valence orbitals show significant variations in the electronic state branching ratios at electron kinetic energies around 60 eV. These features are well reproduced by the present calculations. (C) 1998 Elsevier Science B.V, All rights reserved.
Energy-dependent valence photoelectron spectra of SF6. Ab initio calculations and measurements
Carravetta V;
1998
Abstract
Ab initio calculations of branching ratios and cross-sections for inner- and outer-valence levels of SF6 have been carried out by means of the static exchange (STEX) approximation including full intrachannel interaction. The calculations cover an energy region up to 90 eV for the outer and 130 eV for the inner valence molecular levels and the results are compared with experimental data. It is shown that the molecular orbital static exchange method successfully reproduces the strong multiple resonances in the near continuum. The resonances and the energy dependence of the photoionization cross-sections have been used to settle some assignment problems in the valence photoelectron spectrum of SF6. Photoelectron spectra associated with the 2e(g), 3(1u) and 4a(1g) inner valence orbitals show significant variations in the electronic state branching ratios at electron kinetic energies around 60 eV. These features are well reproduced by the present calculations. (C) 1998 Elsevier Science B.V, All rights reserved.I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.


