Three-dimensional charge density wave observed by angle-resolved photoemission spectroscopy in 1T −VSe2
Source abstract
Abstract
We apply high-resolution angle-resolved photoemission spectroscopy to explore the layered transition-metal dichalcogenide $1T\ensuremath{-}{\mathrm{VSe}}2$ with various photon energies to investigate the three-dimensional (3D) charge-density wave (CDW) transition. Here, we provide quite comprehensive evidence of 3D Fermi surface nesting in $1T\ensuremath{-}{\mathrm{VSe}}2$. The observed Fermi surface (FS) largely overlaps with the in-plane nesting vector reported by the electron-diffraction results. Comparing the CDW gaps below and above ${T}c$, we find that the gaps open along the ellipsoidal FS around the $\overline{M}$ point, in agreement with the in-plane nesting vector. With varying the photon energy, a warping of FS and the nesting condition along ${k}z$ are observed. We further observe the gap variation along the ${k}z$ direction consistent with the out-of-plane nesting conditions. Although it was believed to be a layered two-dimensional material, the satisfaction of the 3D nesting condition of the FS and the variation of gap distribution suggest a 3D character of CDW in $1T\ensuremath{-}{\mathrm{VSe}}2$. Meanwhile, a larger value of $2\mathrm{\ensuremath{\Delta}}/{k}B{T}c$ = 14.76 suggests CDW in $1T\ensuremath{-}{\mathrm{VSe}}2$ beyond the weak-coupling region, the nesting condition and the gap correspondence implies a combined effort in the formation of CDW in this material.
Source: openalex_inverted_index · Quality: baseline
Research context
OpenAlex topics: 2D Materials and Applications · Organic and Molecular Conductors Research · Perovskite Materials and Applications
SciVX discovery tags are terminology-based. OpenAlex topics are source-provided classifications.
References (38)
Show source-provided references
1. 10.1038/nnano.2009.29210.1038/nnano.2009.292 ↗
2. 10.1038/nphoton.2009.16710.1038/nphoton.2009.167 ↗
3. 10.1038/nnano.2012.19310.1038/nnano.2012.193 ↗
4. 10.1038/natrevmats.2017.3310.1038/natrevmats.2017.33 ↗
5. 10.1038/nmat404210.1038/nmat4042 ↗
6. 10.1103/PhysRevB.94.04513110.1103/PhysRevB.94.045131 ↗
7. 10.1103/PhysRevLett.117.10680110.1103/PhysRevLett.117.106801 ↗
8. 10.1038/nnano.2015.14310.1038/nnano.2015.143 ↗
9. 10.1088/0953-8984/23/21/21300110.1088/0953-8984/23/21/213001 ↗
10. 10.1103/PhysRevB.94.12110110.1103/PhysRevB.94.121101 ↗
11. 10.1103/PhysRevB.77.16513510.1103/PhysRevB.77.165135 ↗
12. 10.1088/0305-4608/3/4/02210.1088/0305-4608/3/4/022 ↗
13. 10.1103/PhysRevB.19.342010.1103/PhysRevB.19.3420 ↗
14. 10.1103/PhysRevB.26.575610.1103/PhysRevB.26.5756 ↗
15. 10.1088/0022-3719/19/25/00510.1088/0022-3719/19/25/005 ↗
16. 10.1002/pssa.221074024010.1002/pssa.2210740240 ↗
17. 10.1088/0022-3719/19/3/00610.1088/0022-3719/19/3/006 ↗
18. 10.1103/PhysRevLett.109.08640110.1103/PhysRevLett.109.086401 ↗
19. 10.1143/JPSJ.73.333110.1143/JPSJ.73.3331 ↗
20. 10.1103/PhysRevB.99.11541710.1103/PhysRevB.99.115417 ↗
21. 10.1103/PhysRevB.68.15510810.1103/PhysRevB.68.155108 ↗
22. 10.1021/acs.nanolett.8b0176410.1021/acs.nanolett.8b01764 ↗
23. 10.1016/0038-1098(76)90187-310.1016/0038-1098(76)90187-3 ↗
24. 10.1016/0378-4363(81)90233-310.1016/0378-4363(81)90233-3 ↗
25. 10.1103/PhysRevB.50.1795310.1103/PhysRevB.50.17953 ↗
26. 10.1103/PhysRevB.59.175810.1103/PhysRevB.59.1758 ↗
27. 10.1103/PhysRevB.54.1116910.1103/PhysRevB.54.11169 ↗
28. 10.1103/PhysRevLett.92.24640110.1103/PhysRevLett.92.246401 ↗
29. 10.1103/PhysRevB.82.08110110.1103/PhysRevB.82.081101 ↗
30. 10.1088/0953-8984/22/2/02220110.1088/0953-8984/22/2/022201 ↗
31. 10.1103/PhysRevB.83.19513110.1103/PhysRevB.83.195131 ↗
32. 10.1103/PhysRevB.62.427710.1103/PhysRevB.62.4277 ↗
33. 10.1002/anie.20130433710.1002/anie.201304337 ↗
34. 10.1088/0022-3719/10/14/01310.1088/0022-3719/10/14/013 ↗
35. 10.1002/pssb.222129010310.1002/pssb.2221290103 ↗
36. 10.1063/1.489302710.1063/1.4893027 ↗
37. 10.1103/PhysRevB.101.23540510.1103/PhysRevB.101.235405 ↗
38. 10.1038/s41467-020-20829-210.1038/s41467-020-20829-2 ↗