Share Email Print
cover

Proceedings Paper

Extended x-ray characteristic fluorescence fine structure above the K-edges of Ni, Cu, NiCu, and NiO by fast electron excitation
Author(s): V. Alexandrov; A. Zadorozhny; V. Skudra
Format Member Price Non-Member Price
PDF $14.40 $18.00

Paper Abstract

The extended x-ray fluorescence fine structure (EXFLUFS) above the Ni and Cu K-edge of Ni, Cu, NiCu and NiO using the appearance potential regime by fast electron excitation was measured by means of scanning electron microscope with Si (Li) crystal detector and multichannel analyzer in the raster or single mode. The conventional extended x-ray absorption fine structure (EXAFS) type analysis was made in order to obtain the structural information. The Fourier filtered peak fitting with the phase shift correction from Teo & Lee gives the interatomic distances, which agree well with crystallographic and EXAFS data. The fitting results of experimental data suggest that conventional EXAFS phase shift correction can be safely used for EXFLUFS analysis with a little correction, if needed. The intensities of EXFLUFS peaks differ from that of EXAFS case, probably, because of non-dipole excitation, as well as the elastic scattering of primary electron before and after the inelastic scattering event. The EXFLUFS method is a bulk sensitive method which ensures several orders higher spatial resolution than in the synchrotron x-ray radiation case, as well as allows the deep core excitation in the wide energy range.

Paper Details

Date Published: 6 February 1997
PDF: 5 pages
Proc. SPIE 2968, Optical Organic and Semiconductor Inorganic Materials, (6 February 1997); doi: 10.1117/12.266843
Show Author Affiliations
V. Alexandrov, Institute of Physical Energetics (Latvia)
A. Zadorozhny, Institute of Physical Energetics (Latvia)
V. Skudra, Institute of Physical Energetics (Latvia)


Published in SPIE Proceedings Vol. 2968:
Optical Organic and Semiconductor Inorganic Materials
Edgar A. Silinsh; Arthur Medvids; Andrejs R. Lusis; Andris O. Ozols, Editor(s)

© SPIE. Terms of Use
Back to Top