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High Temperature Thermoelectric Properies of LnPdX (Ln = lanthanide; X = Sb, Bi) Ternary Compounds

Published online by Cambridge University Press:  01 February 2011

Takeyuki Sekimoto
Affiliation:
t-sekimoto@stu.nucl.eng.osaka-u.ac.jp, Osaka University, Yamadaoka 2-1, Suita, Osaka, 565-0871, Japan
Ken Kurosaki
Affiliation:
kurosaki@nucl.eng.osaka-u.ac.jp, Japan
Hiroaki Muta
Affiliation:
muta@nucl.eng.osaka-u.ac.jp, Japan
Shinsuke Yamanaka
Affiliation:
yamanaka@nucl.eng.osaka-u.ac.jp, Japan
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Abstract

Ternary compounds LnPdX (Ln = lanthanide elements of La, Gd, Er; X = Sb, Bi) were prepared by a spark plasma sintering (SPS) technique. The crystal structure of LaPdSb and GdPdSb was confirmed to be a hexagonal ZrBeSi-type structure and different from the other compounds with a MgAgAs-type structure. The electrical resistivities ρ of LaPdSb and GdPdSb indicate the metallic or semimetallic characteristics, while those of ErPdSb and LnPdBi indicate semiconductor characteristics. From the ln ρ − 1/T plot, the band gap energies E g were estimated to be 0.28, 0.053, 0.081, and 0.049 eV for ErPdSb, LaPdBi, GdPdBi, and ErPdBi, respectively. All the samples have positive thermoelectric powers S above room temperature. The largest power factor S 2/ρ was obtained as 49.5 μW/K2 cm at 327 K for LaPdSb. From the Hall effect measurements on ErPdX, the carrier concentration n of ErPdSb and ErPdBi were obtained as 5.9×1018 and 3.21×1019 cm−3 at room temperature, respectively. It is considered that the difference of n at room temperature is mainly due to the magnitude of the band gap energy.

Type
Research Article
Copyright
Copyright © Materials Research Society 2006

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References

REFERENCES

1. Nielsen, J. W. and Baenziger, N. C., Acta. Cryst. 7, 132 (1954).Google Scholar
2. Kaczorowski, D., Gofryk, K., Plackowski, T., Leithe-Jasper, A., and Grin, Yu., Magn, J.. Magn. Mater. 290–291, 573 (2005).Google Scholar
3. Gofryk, K., Kaczorowski, D., Plackowski, T., Leithe-Jasper, A., and Grin, Yu., Phys. Rev. B 72, 094409 (2005).Google Scholar
4. Mastronardi, K., Young, D., Wang, C.-C., Khalifah, P., Cava, R. J., and Ramirez, A. P., Appl. Phys. Lett. 74, 1415 (1999).Google Scholar
5. Cook, B. A. and Harringa, J. L., J. Mater. Sci. 34, 323 (1999).Google Scholar
6. Uher, C., Yang, J., Hu, S., Morelli, D. T., and Meisner, G. P., Phys. Rev. B 59, 8615 (1999).Google Scholar