Magnetism in frustrated Kondo and non-Kondo intermetallics: CeInCu2 versus NdInCu2
Source abstract
Abstract
Single crystalline intermetallics ${\mathrm{CeInCu}}2$ and ${\mathrm{NdInCu}}2$, where the rare earth ions occupy geometrically frustrated fcc lattice of Heusler-type structure, have been studied comparatively to shed light on the ground-state magnetism derived from Kondo physics and/or spin frustration competing with the Ruderman-Kittel-Kasuya-Yosida interaction. ${\mathrm{CeInCu}}2$ is distinct from ${\mathrm{NdInCu}}2$ due to the significant Kondo effect that is absent in the latter. They order antiferromagnetically at ${T}N\phantom{\rule{0.16em}{0ex}}\ensuremath{\approx}\phantom{\rule{0.16em}{0ex}}1.4$ and 2.0 K with large paramagnetic Curie-Weiss temperature of $\ensuremath{-}35.4$ K and $\ensuremath{-}41.1$ K, respectively. The electronic specific-heat coefficient $\ensuremath{\gamma}$ = $C/T$ ($T\phantom{\rule{0.16em}{0ex}}\ensuremath{\rightarrow}\phantom{\rule{0.16em}{0ex}}0$) = 870 mJ ${\mathrm{mol}}^{\ensuremath{-}1}\phantom{\rule{4pt}{0ex}}{\mathrm{K}}^{\ensuremath{-}2}$ in ${\mathrm{CeInCu}}2$ is significantly enhanced, much larger than 180 mJ ${\mathrm{mol}}^{\ensuremath{-}1}\phantom{\rule{4pt}{0ex}}{\mathrm{K}}^{\ensuremath{-}2}$ of the latter that is also enhanced albeit its non-Kondo nature. For both compounds, the Kadowaki-Woods ratio deviates greatly from the standard value expected from a Kramers doublet ground state, which, however, can be restored if one considers a smaller but still sizable $\ensuremath{\gamma}$ estimated from the paramagnetic state. Likewise, the Kondo temperature of ${\mathrm{CeInCu}}2$ is revised to be ${T}K\phantom{\rule{4pt}{0ex}}\ensuremath{\approx}$ 13 K that is double the literature values, manifesting a major effect of spin frustration to low-temperature thermodynamics beyond the Kondo physics. Similarities between the two compounds is also noticed in their temperature-field phase diagrams in spite of their thermodynamic distinctions in the thermal expansion and the Gr\"uneisen ratio, which are much more sensitive to Kondo hybridization than to geometrical frustration.
Source: openalex_inverted_index · Quality: baseline
Research context
OpenAlex topics: Rare-earth and actinide compounds · Iron-based superconductors research · Inorganic Chemistry and Materials
SciVX discovery tags are terminology-based. OpenAlex topics are source-provided classifications.
References (38)
Show source-provided references
1. 10.1103/RevModPhys.56.75510.1103/RevModPhys.56.755 ↗
2. 10.1038/nphys89210.1038/nphys892 ↗
3. 10.1002/pssb.20098308210.1002/pssb.200983082 ↗
4. 10.1007/s10909-010-0213-410.1007/s10909-010-0213-4 ↗
5. 10.1038/s41567-019-0666-610.1038/s41567-019-0666-6 ↗
6. 10.1103/PhysRevB.100.02440410.1103/PhysRevB.100.024404 ↗
7. 10.1103/PhysRevResearch.2.01318310.1103/PhysRevResearch.2.013183 ↗
8. 10.1016/0038-1098(85)90392-810.1016/0038-1098(85)90392-8 ↗
9. 10.1007/BF0130397910.1007/BF01303979 ↗
10. 10.1016/0304-8853(87)90536-110.1016/0304-8853(87)90536-1 ↗
11. 10.1088/0305-4608/17/12/01310.1088/0305-4608/17/12/013 ↗
12. 10.1143/JPSJ.57.156210.1143/JPSJ.57.1562 ↗
13. 10.1016/0304-8853(88)90396-410.1016/0304-8853(88)90396-4 ↗
14. 10.1143/JPSJ.57.227610.1143/JPSJ.57.2276 ↗
15. 10.1143/JPSJ.58.429210.1143/JPSJ.58.4292 ↗
16. 10.1103/PhysRevB.81.17441310.1103/PhysRevB.81.174413 ↗
17. 10.1016/0304-8853(83)90298-610.1016/0304-8853(83)90298-6 ↗
18. 10.1143/JPSJ.32.124810.1143/JPSJ.32.1248 ↗
19. 10.1016/0304-8853(92)90652-510.1016/0304-8853(92)90652-5 ↗
20. 10.1016/j.physc.2007.03.12110.1016/j.physc.2007.03.121 ↗
21. 10.1088/1742-6596/683/1/01201710.1088/1742-6596/683/1/012017 ↗
22. 10.1016/0921-4526(93)90640-R10.1016/0921-4526(93)90640-R ↗
23. 10.1016/0375-9601(82)90481-910.1016/0375-9601(82)90481-9 ↗
24. 10.1103/PhysRevLett.51.30810.1103/PhysRevLett.51.308 ↗
25. 10.1038/nphys94210.1038/nphys942 ↗
26. 10.1103/PhysRevB.94.23513110.1103/PhysRevB.94.235131 ↗
27. 10.1103/PhysRevB.77.06443210.1103/PhysRevB.77.064432 ↗
28. 10.1143/JPSJ.59.345110.1143/JPSJ.59.3451 ↗
29. 10.1007/BF0130445810.1007/BF01304458 ↗
30. 10.1103/PhysRevB.68.18441910.1103/PhysRevB.68.184419 ↗
31. 10.1103/PhysRevB.61.892210.1103/PhysRevB.61.8922 ↗
32. 10.1088/1742-6596/150/4/04213910.1088/1742-6596/150/4/042139 ↗
33. 10.1088/0034-4885/79/11/11450210.1088/0034-4885/79/11/114502 ↗
34. 10.1016/0038-1098(86)90785-410.1016/0038-1098(86)90785-4 ↗
35. 10.1103/PhysRevLett.94.05720110.1103/PhysRevLett.94.057201 ↗
36. 10.1088/1674-1056/ac0a6010.1088/1674-1056/ac0a60 ↗
37. 10.1103/PhysRevLett.119.12640210.1103/PhysRevLett.119.126402 ↗
38. 10.1038/s41586-020-2052-z10.1038/s41586-020-2052-z ↗