Figure9

EXAFS spectroscopy: a powerful tool for the study of local vibrational dynamics

Figure 9. Temperature dependence of ΔC2 (squares) and best fit using the correlated Einstein model (dashed line), which gives ν=13.1 THz and a constant shift |a|=0.0036Å2. Circles and solid line are, respectively, the resulting parallel MSRD and the corresponding Einstein model. Error bars have been omitted for clarity.

Microstructures
ISSN 2770-2995 (Online)

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