Abstract
A theory combining Hellmann–Feynman electrostatic forces and one-electron molecular orbital energies is used to determine spectroscopic properties for diatomic and surface nickel chalcogenides. The small cluster model for the surface is found adequate for all properties considered. The absorbate p photoemission bands are interpreted in terms of final-state chalcogen atom multiplet splittings, opposed to previous studies which attributed the complicated spectra to unusual bonding interactions between the absorbate and substrate.

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