Abstract
Classical molecular dynamics (MD) and reverse Monte Carlo methods coupled with ab initio multiple-scattering extended x-ray absorption fine structure (EXAFS) calculations were used for modeling of scheelite-type AWO4 (A = Ca, Sr, Ba) W L 3-edge EXAFS spectra. The two theoretical approaches are complementary and allowed us to perform analysis of full EXAFS spectra. Both methods reproduce well the structure and dynamics of tungstates in the outer coordination shells, however the classical MD simulations underestimate the W-O bond MSRD due to a neglect of quantum zero-point-motion. The thermal vibration amplitudes, correlation effects and anisotropy of the tungstate structure were also estimated.
| Original language | English |
|---|---|
| Article number | 114001 |
| Journal | Physica Scripta |
| Volume | 91 |
| Issue number | 11 |
| DOIs | |
| Publication status | Published - 18 Oct 2016 |
Keywords
- EXAFS
- molecular dynamics
- reverse Monte Carlo
- tungstates
- W L3-edge
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