Improved Figure of Merit of Cu2SnSe3 via Band Structure Modification and Energy-Dependent Carrier Scattering
Source abstract
Abstract
As an ecofriendly thermoelectric material with intrinsic low thermal conductivity, ternary diamond-like Cu2SnSe3 (CSS) has attracted much attention. Nevertheless, its figure of merit, ZT, is limited by its small thermopower (S) and power factor (PF). Here, we show that an increase in thermopower by 63% and a carrier-mobility rise of 81% at 300 K can be simultaneously achieved through 5% substitution of Fe for Sn due to both enhancement of electronic density of states and degeneracy of multiple valence band maxima, which lead to high PF = 10.3 μW·cm–1·K–2 at 823 K for Fe-doped CSS (CSFS). Besides, an ultrahigh PF of 14.8 μW·cm–1·K–2 (at 773 K) and 45% reduction of lattice thermal conductivity (at 823 K) are realized for CSFS-based composites with 0.125 wt % of MgO nanoinclusions, owing to further enhancement of S via energy-dependent scattering and strong phonon scattering by the embedded nanoparticles. Consequently, a maximum ZT = 1 at 823 K is reached for the CSFS/f MgO composite samples with f = 0.125 wt %, which is around 2.5 times larger than that of the CSS compound.
Source: openalex_inverted_index · Quality: baseline
Research context
OpenAlex topics: Advanced Thermoelectric Materials and Devices · Chalcogenide Semiconductor Thin Films · 2D Materials and Applications
SciVX discovery tags are terminology-based. OpenAlex topics are source-provided classifications.
Affiliations
Key Laboratory of Material Physics, Institute of Solid State Physics, Chinese Academy of Sciences, 230031 Hefei, PR China
University of Science and Technology of China, 230026 Hefei, PR China
MIT Key Laboratory of Advanced Metalic and Intermetallic Materials Technology, Nanjing University of Science and Technology, 210094 Nanjing, PR China
Funding
National Natural Science Foundation of China
References (39)
Show source-provided references
1. 10.1126/science.115889910.1126/science.1158899 ↗
2. 10.1016/j.mtphys.2019.10009610.1016/j.mtphys.2019.100096 ↗
3. 10.1021/jacs.8b0937510.1021/jacs.8b09375 ↗
4. 10.1002/adma.20170314810.1002/adma.201703148 ↗
5. 10.1038/nature0999610.1038/nature09996 ↗
6. 10.1126/science.115972510.1126/science.1159725 ↗
7. 10.1021/acsaem.9b0206110.1021/acsaem.9b02061 ↗
8. 10.1016/j.mtphys.2019.03.00510.1016/j.mtphys.2019.03.005 ↗
9. 10.1039/c9ta05798f10.1039/c9ta05798f ↗
10. 10.1039/c3ta15211a10.1039/c3ta15211a ↗
11. 10.1002/adma.20190521010.1002/adma.201905210 ↗
12. 10.1021/acsami.9b2010310.1021/acsami.9b20103 ↗
13. 10.1021/jacs.6b0701010.1021/jacs.6b07010 ↗
14. 10.1021/jacs.7b1187510.1021/jacs.7b11875 ↗
15. 10.1126/science.aax512310.1126/science.aax5123 ↗
16. 10.1063/1.511940210.1063/1.5119402 ↗
17. 10.1016/j.scriptamat.2017.12.03510.1016/j.scriptamat.2017.12.035 ↗
18. 10.1002/adfm.20160148610.1002/adfm.201601486 ↗
19. 10.1021/ic401317k10.1021/ic401317k ↗
20. 10.1021/cm101589c10.1021/cm101589c ↗
21. 10.1021/acsami.9b0134810.1021/acsami.9b01348 ↗
22. 10.1016/j.scriptamat.2018.09.01010.1016/j.scriptamat.2018.09.010 ↗
23. 10.1038/srep1780310.1038/srep17803 ↗
24. 10.1103/physrevb.54.1116910.1103/physrevb.54.11169 ↗
25. 10.1103/physrevb.50.1795310.1103/physrevb.50.17953 ↗
26. 10.1103/physrevlett.77.386510.1103/physrevlett.77.3865 ↗
27. 10.1002/pssb.20140034610.1002/pssb.201400346 ↗
28. 10.1103/physrevb.86.15520110.1103/physrevb.86.155201 ↗
29. 10.1016/j.materresbull.2003.09.01710.1016/j.materresbull.2003.09.017 ↗
30. 10.1007/s00339-017-1540-y10.1007/s00339-017-1540-y ↗
31. 10.1063/1.494199910.1063/1.4941999 ↗
32. 10.1016/j.jallcom.2015.11.21710.1016/j.jallcom.2015.11.217 ↗
33. 10.1016/j.jallcom.2012.12.04810.1016/j.jallcom.2012.12.048 ↗
34. 10.1103/physrevb.70.11533410.1103/physrevb.70.115334 ↗
35. 10.1063/1.486115610.1063/1.4861156 ↗
36. 10.1063/1.480185110.1063/1.4801851 ↗
37. 10.1039/c7ta02178j10.1039/c7ta02178j ↗
38. 10.1021/acsnano.6b0115610.1021/acsnano.6b01156 ↗
39. 10.1103/physrev.113.104610.1103/physrev.113.1046 ↗