4.6 Article

Next-nearest neighbour contributions to the XPS binding energies and XANES absorption energies of P and As in transition-metal arsenide phosphides MAs1-yPy having the MnP-type structure

Journal

JOURNAL OF SOLID STATE CHEMISTRY
Volume 181, Issue 10, Pages 2549-2558

Publisher

ACADEMIC PRESS INC ELSEVIER SCIENCE
DOI: 10.1016/j.jssc.2008.06.034

Keywords

XPS; XANES Next-nearest neighbour shift; Charge potential model; Phosphides; Arsenides

Funding

  1. Natural Sciences and Engineering Research Council (NSERC) of Canada
  2. Alberta Centre for Surface Engineering and Science (AGES) at the University of Alberta
  3. Canada Foundation for Innovation (CFI)
  4. US Department of Energy-Basic Energy Sciences [DE-AC02-06CH11357]
  5. NSERC
  6. University of Washington
  7. Simon Fraser University
  8. APS
  9. University of Alberta

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X-ray photoelectron spectroscopic (XPS) and X-ray absorption near-edge spectroscopic (XANES) measurements have been made for several series of metal arsenide phosphides MAs1-yPy (M = Co, Fe, Cr) that adopt the MO-type Structure. The P and As XPS binding energies (BEs) and XANES absorption energies of the metal arsenide phosphides do not follow the trend observed for the simple binary phosphides or arsenides, a deviation that arises from the combination of nearest and next-nearest neighbour contributions acting oil the 13 or As photoemission or absorption site. The P 2p(3/2) BEs and K-edge absorption energies are lower in MAs1-yPy than in MP because the P atoms are more negatively charged and because the P photoemission or absorption site is screened to a greater extent by less positively charged nearest-neighbour M atoms and more negatively charged next-nearest neighbour P atoms. The As L-3- and K-edge absorption energies are higher in MAs1-yPy than in MAs primarily because the As atoms are less negatively charged. The M charge has been evaluated from analysis of the M 2p XPS spectra and the M L- and K-edge XANES spectra. (c) 2008 Elsevier Inc. All rights reserved.

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