Abstract
After performing first-principles calculations of structural and vibrational properties of
the semiconducting clathrates Rb24Ga24Sn112 along with binary CsxSn136 (0 x 24), we obtained
equilibrium geometries and harmonic phonon modes. For the filled clathrate Rb24Ga24Sn112, the
phonon dispersion relation predicts an upshift of the low-lying rattling modes (~25 cm1) for
the Rb (“rattler”) compared to Cs vibration in CsxSn136. It is also found that the large isotropic
atomic displacement parameter (Uiso) exists when Rb occupies the “over-sized” cage (28 atom cage)
rather than the 20 atom counterpart. These guest modes are expected to contribute significantly to
minimizing the lattice’s thermal conductivity (L). Our calculation of the vibrational contribution to
the specific heat and our evaluation on L are quantitatively presented and discussed. Specifically,
the heat capacity diagram regarding CV/T3 vs. T exhibits the Einstein-peak-like hump that is mainly
attributable to the guest os
Original language | English |
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Pages (from-to) | 74-91 |
Journal | Inorganics |
State | Published - Jun 19 2019 |