Large thermopower from dressed quasiparticles in the layered cobaltates and rhodates
Source abstract
Abstract
The origin of the large thermopower in ${\mathrm{Na}}x{\mathrm{CoO}}2$ is complicated by correlation phenomena. To disentangle the effects from multiple interactions, we use angle-resolved photoemission to study ${\mathrm{K}}x{\mathrm{RhO}}2$, an isostructural analogy of ${\mathrm{Na}}x{\mathrm{CoO}}2$ with large thermopower and weak electron correlation. Using the experimentally measured electronic structure, we demonstrate that the thermopower in ${\mathrm{K}}x{\mathrm{RhO}}2$ can be quantitatively explained within the quasiparticle framework after including an electron-phonon mass enhancement effect. Extending the analysis to the cobaltate, we find the doubling in thermopower is well accounted for by additional band renormalization from electron correlation. As such, the large thermopower emerges from the itinerant quasiparticles dressed by hierarchical electron-phonon and electron-electron interactions.
Source: openalex_inverted_index · Quality: baseline
Research context
OpenAlex topics: Advanced Thermoelectric Materials and Devices · Thermal Expansion and Ionic Conductivity · Magnetic and transport properties of perovskites and related materials
SciVX discovery tags are terminology-based. OpenAlex topics are source-provided classifications.
References (40)
Show source-provided references
1. 10.1557/jmr.2011.10810.1557/jmr.2011.108 ↗
2. 10.1103/PhysRevB.56.R1268510.1103/PhysRevB.56.R12685 ↗
3. 10.1038/nmat166910.1038/nmat1669 ↗
4. 10.1103/PhysRevB.59.945410.1103/PhysRevB.59.9454 ↗
5. 10.1038/nature0163910.1038/nature01639 ↗
6. 10.1103/PhysRevLett.92.24700110.1103/PhysRevLett.92.247001 ↗
7. 10.1103/PhysRevLett.94.15720610.1103/PhysRevLett.94.157206 ↗
8. 10.1103/PhysRevLett.94.15720510.1103/PhysRevLett.94.157205 ↗
9. 10.1103/PhysRevLett.96.04640710.1103/PhysRevLett.96.046407 ↗
10. 10.1038/nature0145010.1038/nature01450 ↗
11. 10.1103/PhysRevB.13.64710.1103/PhysRevB.13.647 ↗
12. 10.1103/PhysRevB.62.686910.1103/PhysRevB.62.6869 ↗
13. 10.1103/PhysRevLett.87.23660310.1103/PhysRevLett.87.236603 ↗
14. 10.1103/PhysRevLett.93.05640110.1103/PhysRevLett.93.056401 ↗
15. 10.1103/PhysRevB.61.1339710.1103/PhysRevB.61.13397 ↗
16. 10.1103/PhysRevB.69.12541010.1103/PhysRevB.69.125410 ↗
17. 10.1143/JPSJ.76.08370710.1143/JPSJ.76.083707 ↗
18. 10.1103/PhysRevLett.92.24640210.1103/PhysRevLett.92.246402 ↗
19. 10.1103/PhysRevLett.92.24640310.1103/PhysRevLett.92.246403 ↗
20. 10.1103/PhysRevLett.94.20640110.1103/PhysRevLett.94.206401 ↗
21. 10.1103/PhysRevLett.95.14640110.1103/PhysRevLett.95.146401 ↗
22. 10.1103/PhysRevLett.97.18640510.1103/PhysRevLett.97.186405 ↗
23. 10.1103/PhysRevLett.99.04640310.1103/PhysRevLett.99.046403 ↗
24. 10.1088/0953-8984/22/11/11560310.1088/0953-8984/22/11/115603 ↗
25. 10.1063/1.476746410.1063/1.4767464 ↗
26. 10.1103/PhysRevB.84.07511010.1103/PhysRevB.84.075110 ↗
27. 10.1002/adfm.20110310610.1002/adfm.201103106 ↗
28. 10.1103/PhysRevLett.96.21640510.1103/PhysRevLett.96.216405 ↗
29. 10.1103/PhysRevLett.106.07700510.1103/PhysRevLett.106.077005 ↗
30. 10.1103/PhysRev.129.13810.1103/PhysRev.129.138 ↗
31. 10.1103/PhysRevLett.101.06640310.1103/PhysRevLett.101.066403 ↗
32. 10.1103/PhysRevLett.102.06640210.1103/PhysRevLett.102.066402 ↗
33. 10.1103/PhysRevLett.97.01640410.1103/PhysRevLett.97.016404 ↗
34. 10.1063/1.492838410.1063/1.4928384 ↗
35. 10.1088/1367-2630/13/4/04302110.1088/1367-2630/13/4/043021 ↗
36. 10.1103/PhysRevB.79.07510510.1103/PhysRevB.79.075105 ↗
37. 10.1103/PhysRevB.76.19511110.1103/PhysRevB.76.195111 ↗
38. 10.1103/PhysRevB.42.935010.1103/PhysRevB.42.9350 ↗
39. 10.1103/PhysRevLett.104.05640310.1103/PhysRevLett.104.056403 ↗
40. 10.1103/PhysRevLett.102.02680610.1103/PhysRevLett.102.026806 ↗