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Hamawandi et al. Energy Mater. 2025, 5, 500065  https://dx.doi.org/10.20517/energymater.2024.204  Page 11 of 20



























                                                                   2
                Figure 6. Temperature dependence of the experimental EXAFS spectra [χ(k)k ] and their Fourier transforms (FTs) for the Sb and Te K-
                edges in Sb Te  (A and B) and Bi L -edge and Te K-edge in Bi Te  (C and D). The FTs were calculated in the k-space range of
                        2  3            3                   2  3
                       -1
                3.0-15.4 Å , and only the FT modulus is shown for clarity.




































                Figure 7. Temperature-dependent radial distribution functions (RDFs) g(r) calculated from the results of RMC/EA simulations for
                Sb Te  (A and B) and Bi Te  (C and D). Vertical lines show calculated average interatomic distances at 10 K (blue) and 300 K (red).
                                2
                                  3
                   3
                 2
                The nearest atom pairs are indicated for clarity. The Te2-Te2 atom pairs from different layers are highlighted in red.
               and from about 3.24 to 3.26 Å in Bi Te  when heated from 10 up to 300 K. The Bi-Te interatomic distances
                                             2
                                                3
               are larger relative to Sb-Te due to differences in the radii of Bi and Sb atoms. Indeed, the ionic radius of
               sixfold coordinated Bi  (1.03 Å) is larger than that of Sb  (0.76 Å) . Notably, both Sb Te  and Bi Te
                                                                           [52]
                                   3+
                                                                  3+
                                                                                                       2
                                                                                                         3
                                                                                             2
                                                                                                3
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