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Phys. Rev. B 21, 2108–2121 (1980)

Effect of the central atom potential on the extended fine structure above appearance potential thresholds

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G. E. Laramore
Department of Radiation Oncology, University of Washington Hospital, Seattle, Washington 98195

T. L. Einstein, L. D. Roelofs, and Robert L. Park
Department of Physics and Astronomy, University of Maryland, College Park, Maryland 20742

Received 5 September 1979; published in the issue dated 15 March 1980

The formalism previously given for describing the extended fine structure above appearance-potential-spectroscopy (APS) thresholds is extended by incorporating the effects of the excited "central" atom potential in an exact manner. The excitation-matrix elements are expressed in terms of the exact wave functions of the central atom potential. This introduces a "phase renormalization" into the excitation-matrix elements and eliminates a previously noted "phase difference" between single- and multiple-scattering calculations employing a plane-wave basis set. A series of approximations is then made which leads to an expression for the APS extended fine structure in terms of sinusoidal functions and hence provides a rationale for a Fourier-transform analysis. Simple model calculations assuming a constant "bare" excitation-matrix element, a spherically symmetric electronic density of states, and only S-wave scattering from the atomic cores are performed for a cluster of atoms having the atomic geometry of bulk vanadium. These calculations display the major predictions of the formalism and indicate that for a given system there may be some optimal energy range for data analysis. The problem of electron characteristic losses is considered, and it is pointed out that in the small-momentum-transfer limit the simple dipole selection rules appropriate to a photon-excitation process again apply. This may obviate many of the problems introduced by multiple angular momentum final states in the APS process.

© 1980 The American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevB.21.2108
DOI:
10.1103/PhysRevB.21.2108
PACS: