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Published November 10, 2015 | Supplemental Material
Journal Article Open

Coinage-Metal-Stuffed Eu_9Cd_4Sb_9: Metallic Compounds with Anomalous Low Thermal Conductivities

Abstract

The synthesis and transport properties of the family of coinage metal-stuffed Zintl compounds, Eu_9Cd_(4–x)CM_(2+x–y□y)Sb_9 (CM = coinage metal, □ = vacancies), is presented as a function of coinage metal substitution. Eu_9Cd_(4–x)CM_(2+x–y□y)Sb_9 compounds are shown to be rare examples of metallic Zintl phases with low thermal conductivities. While the lattice thermal conductivity is low, which is attributed to the complex structure and presence of interstitials, the electronic contribution to thermal conductivity is also low. In these p-type compounds, the carriers transmit less heat than expected, based on the Wiedemann–Franz law and metallic conduction, κ_e = L_0T/ρ. Density functional theory (DFT) calculations indicate that the Fermi level resides in a pseudo-gap, which is consistent with the metallic description of the properties. While the contribution from the interstitial CM states to the Fermi level is small, the interstitial CMs are required to tune the position of the Fermi level. Analysis of the topology of electron localization function (ELF) basins reveals the multicenter Eu−Cd(CM)−Sb interactions, as the Eu and Sb states have the largest contribution at the top of the valence band. Regardless of the success of the Zintl concept in the rationalization of the properties, the representation of the CM-stuffed Eu_9Cd_4Sb_9 structure as Eu cations encapsulated into a polyanionic (Cd/Cu)Sb network is oversimplified and underestimates the importance of the Eu–Sb bonding interactions. These results provide motivation to search for more efficient thermoelectric materials among complex metallic structures that can offer less electronic thermal conductivity without deteriorating the electrical conductivity.

Additional Information

© 2015 American Chemical Society. Received: September 27, 2015; Revised: October 12, 2015; Published: October 14, 2015. We thank Dr. Sarah Roeske and Nick Botto for assistance with microprobe analysis. We also thank Kathleen Lee for assistance with the thermal conductivity measurements under the magnetic field and Prof. Kovnir for use of the PPMS. This research was funded by a Summer GSR and Ernest E. Hill fellowships for N.K. and the National Science Foundation (NSF) (Grant No. DMR-1405973). G.J.S. and S.O. were supported by the NASA Science Missions Directorate's Radioisotope Power Systems Technology Advancement Program through NASA/JPL. The authors declare no competing financial interest.

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August 20, 2023
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