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通过Sb-Sn无序和相分离促进,Sn掺杂稀土(M)填充方钴矿MCoSbSn中晶格热导率大幅降低。

Strongly reduced lattice thermal conductivity in Sn-doped rare-earth (M) filled skutterudites M CoSb Sn , promoted by Sb-Sn disordering and phase segregation.

作者信息

Gainza J, Serrano-Sánchez F, Nemes N M, Dura O J, Martínez J L, Fauth F, Alonso J A

机构信息

Instituto de Ciencia de Materiales de Madrid (ICMM), Consejo Superior de Investigaciones Científicas (CSIC), Sor Juana Inés de la Cruz 3 E-28049 Madrid Spain

Departamento de Física de Materiales, Universidad Complutense de Madrid E-28040 Madrid Spain.

出版信息

RSC Adv. 2021 Aug 3;11(42):26421-26431. doi: 10.1039/d1ra04270j. eCollection 2021 Jul 27.

Abstract

CoSb thermoelectric skutterudite has been filled with rare-earth metals (M = La, Ce, Yb) and partially doped with Sn in specimens of M CoSb Sn stoichiometry. This has been achieved under high-pressure conditions at 3.5 GPa in a piston-cylinder hydrostatic press. A structural investigation using synchrotron X-ray diffraction data reveals a phase segregation in twin skutterudite phases with filling fraction fluctuation and different unit-cell sizes. As a result of three effects acting as phonon scatterers, namely the rattling effect of M at the wide 8 cages of the cubic 3̄ structure, the phase segregation, and the intrinsic disorder introduced by Sn substitution at the Sb sublattice, the total thermal conductivity () dramatically falls to reach minimum values under 2 W m K, well below those typically exhibited by other thermoelectric materials based upon single-filled skutterudites. The power factor is substantially enhanced to 1.11 mW m K in YbCoSbSn with respect to the unfilled composition, as a result of the charge transfer promoted by the filler.

摘要

在具有M-CoSb-Sn化学计量比的样品中,CoSb热电方钴矿已用稀土金属(M = La、Ce、Yb)填充并部分掺杂了Sn。这是在活塞-圆筒静水压力机中3.5 GPa的高压条件下实现的。利用同步加速器X射线衍射数据进行的结构研究揭示了在孪晶方钴矿相中存在相分离,其填充率存在波动且晶胞尺寸不同。由于三种作为声子散射体的效应,即M在立方3̄结构的宽8笼中的晃动效应、相分离以及Sn在Sb亚晶格处取代引入的本征无序,总热导率()急剧下降,达到低于2 W m⁻¹K⁻¹的最小值,远低于其他基于单填充方钴矿的热电材料通常表现出的值。由于填充剂促进了电荷转移,相对于未填充的成分,YbCoSbSn中的功率因数大幅提高到1.11 mW m⁻¹K⁻²。

https://cdn.ncbi.nlm.nih.gov/pmc/blobs/c396/9037351/d78d6913eeb8/d1ra04270j-f1.jpg

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