Charge density wave and lock-in transitions of CuV2S4
Source abstract
Abstract
The three-dimensional charge density wave (CDW) compound ${\mathrm{CuV}}2{\mathrm{S}}4$ is known to undergo phase transitions at $\ensuremath{\sim}91$ and $\ensuremath{\sim}50\phantom{\rule{4pt}{0ex}}\mathrm{K}$. Employing single-crystal x-ray diffraction on an annealed crystal, we confirm the formation of an incommensurate CDW at ${T}_{\text{CDW}}\ensuremath{\approx}91\phantom{\rule{4pt}{0ex}}\mathrm{K}$, and we establish the nature of the transition at ${T}_{\text{lock-in}}\ensuremath{\approx}50\phantom{\rule{4pt}{0ex}}\mathrm{K}$ as a lock-in transition toward a threefold superstructure. As-grown crystals develop the same incommensurate CDW as the annealed crystal does, but they fail to go through the lock-in transition. Instead, the length of the modulation wave vector continues to decrease down to low temperatures in as-grown crystals. These findings are corroborated by distinct temperature dependencies of the electrical resistivity, magnetic susceptibility, and specific heat measured on as-grown and annealed crystals. A superspace model for the crystal structure of the incommensurate CDW suggests that the formation of extended vanadium clusters is at the origin of the CDW. In the lock-in phase, short and long V-V distances persist, but clusters now percolate the entire crystal. The lowering toward orthorhombic symmetry appears to be responsible for the precise pattern of short and long V-V distances. However, the orthorhombic lattice distortion is nearly zero for the annealed crystal, while it is visible for the as-grown material, again suggesting the role of lattice defects in the latter.
Source: openalex_inverted_index · Quality: baseline
Research context
OpenAlex topics: Organic and Molecular Conductors Research · Electronic and Structural Properties of Oxides · Advanced Condensed Matter Physics
SciVX discovery tags are terminology-based. OpenAlex topics are source-provided classifications.
References (35)
Show source-provided references
1. G. Gruner · 1994
2. 10.1080/00018732.2012.71967410.1080/00018732.2012.719674 ↗
3. 1996
4. 10.1016/0038-1098(76)90289-110.1016/0038-1098(76)90289-1 ↗
5. 10.1103/PhysRevB.77.16513510.1103/PhysRevB.77.165135 ↗
6. 10.1073/pnas.142479111210.1073/pnas.1424791112 ↗
7. 10.1038/nphys326710.1038/nphys3267 ↗
8. 10.1088/0034-4885/79/8/08450510.1088/0034-4885/79/8/084505 ↗
9. 10.1088/1361-6633/aa7d5f10.1088/1361-6633/aa7d5f ↗
10. 10.1103/PhysRevLett.102.07640410.1103/PhysRevLett.102.076404 ↗
11. 10.1103/PhysRevB.93.16510810.1103/PhysRevB.93.165108 ↗
12. 10.1103/PhysRevB.95.23515610.1103/PhysRevB.95.235156 ↗
13. 10.1103/PhysRevB.97.04110310.1103/PhysRevB.97.041103 ↗
14. 10.1103/PhysRevB.94.07510910.1103/PhysRevB.94.075109 ↗
15. 10.1103/PhysRevB.91.16514110.1103/PhysRevB.91.165141 ↗
16. 10.1038/srep4088610.1038/srep40886 ↗
17. 10.1088/0953-8984/19/21/21621010.1088/0953-8984/19/21/216210 ↗
18. 10.1103/PhysRevB.34.459010.1103/PhysRevB.34.4590 ↗
19. 10.1038/nphys36010.1038/nphys360 ↗
20. 10.1103/PhysRevB.26.250110.1103/PhysRevB.26.2501 ↗
21. 10.1103/PhysRevB.24.285010.1103/PhysRevB.24.2850 ↗
22. 10.1143/JPSJ.73.322710.1143/JPSJ.73.3227 ↗
23. 10.7566/JPSJ.82.06460310.7566/JPSJ.82.064603 ↗
24. 10.1016/0022-4596(87)90319-710.1016/0022-4596(87)90319-7 ↗
25. 10.1016/j.jmmm.2003.11.18310.1016/j.jmmm.2003.11.183 ↗
26. 10.1524/ncrs.1998.213.14.1210.1524/ncrs.1998.213.14.12 ↗
27. 10.1107/S160057751600241110.1107/S1600577516002411 ↗
28. 10.1088/1742-6596/425/1/01201510.1088/1742-6596/425/1/012015 ↗
29. 2002
30. 10.1107/S010876731004229710.1107/S0108767310042297 ↗
31. A. G. Jackson · 199110.1007/978-1-4612-3052-6 ↗
32. 10.1515/zkri-2014-173710.1515/zkri-2014-1737 ↗
33. 10.1103/PhysRevB.53.962610.1103/PhysRevB.53.9626 ↗
34. 10.1103/PhysRevB.64.11511610.1103/PhysRevB.64.115116 ↗
35. 10.1103/PhysRevB.82.05412010.1103/PhysRevB.82.054120 ↗