journal article·2024-04-09

Symmetry breaking and structural instability in ultrathin 2H−TaS2 across the charge density wave transition

Divya Rawat, Aksa Thomas, Ajay Partap Singh Rana, Chandan Bera, Ajay Soni

Physical Review B· Volume 109· Issue 15
Publisher page

Abstract

Ultrathin two-dimensional materials have shown a complete paradigm shift for understanding of physical and electronic properties because of quantum confinement effects and symmetry breaking at nanoscale. Bulk $2H\text{\ensuremath{-}}\mathrm{Ta}{\mathrm{S}}2$ undergoes an incommensurate charge density wave (I-CDW) at temperature ${T}_{\mathrm{I}\ensuremath{-}\mathrm{CDW}}\ensuremath{\sim}76$ K, however, the onset of CDW in atomically thin layers is not clear. We have explored the CDW instability in exfoliated $2H\text{\ensuremath{-}}\mathrm{Ta}{\mathrm{S}}2$ using low temperature polarized Raman spectroscopy and first principles calculation. We have emphasized CDW associated modes, ${M}1\ensuremath{\sim}125 \mathrm{c}{\mathrm{m}}^{\ensuremath{-}1}$ (${E}1$), ${M}2\ensuremath{\sim}158 \mathrm{c}{\mathrm{m}}^{\ensuremath{-}1}$ (${A}1$), and ${M}3\ensuremath{\sim}334 \mathrm{c}{\mathrm{m}}^{\ensuremath{-}1}$ (${E}2$), in the ultrathin layer of a single unit cell with thickness $d\ensuremath{\sim}3$ nm. The asymmetric Fano line shape of ${M}2$ and its anomalous behavior suggests strong electron-phonon coupling, which mainly drives the CDW instability in $2H\text{\ensuremath{-}}\mathrm{Ta}{\mathrm{S}}2$. Our observations provide key evidence that CDW can persist even in one unit cell with a ${T}_{\mathrm{I}\ensuremath{-}\mathrm{CDW}}\ensuremath{\sim}200$ K, which is much higher than bulk $2H\text{\ensuremath{-}}\mathrm{Ta}{\mathrm{S}}2$, and the results are supported by density functional theory.
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Research context

OpenAlex topics: 2D Materials and Applications · Organic and Molecular Conductors Research · Electronic and Structural Properties of Oxides

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Affiliations

School of Physical Sciences, Indian Institute of Technology Mandi, Mandi 175005, Himachal Pradesh, India

Institute of Nano Science and Technology, Sector-81, Knowledge City, Sahibzada Ajit Singh Nagar, 140306, Punjab, India

Funding

Indian Institute of Technology Mandi · Nanoscience and Technology Mohali

References (51)

Show source-provided references
1. 10.1007/s12274-016-1034-910.1007/s12274-016-1034-9 ↗
2. 10.1002/adma.20190700610.1002/adma.201907006 ↗
3. 10.1021/nn400280c10.1021/nn400280c ↗
4. 10.1021/acsnano.9b0341910.1021/acsnano.9b03419 ↗
5. 10.1103/PhysRevLett.125.18640110.1103/PhysRevLett.125.186401 ↗
6. 10.1038/s41467-020-15715-w10.1038/s41467-020-15715-w ↗
7. 10.1103/PhysRevResearch.2.03311810.1103/PhysRevResearch.2.033118 ↗
8. 10.1021/nl504811s10.1021/nl504811s ↗
9. 10.1038/nnano.2015.14310.1038/nnano.2015.143 ↗
10. 10.1038/nnano.2014.32310.1038/nnano.2014.323 ↗
11. 10.1103/RevModPhys.60.112910.1103/RevModPhys.60.1129 ↗
12. 10.1103/PhysRevLett.32.88210.1103/PhysRevLett.32.882 ↗
13. 10.1103/PhysRevB.99.17411010.1103/PhysRevB.99.174110 ↗
14. 10.1103/PhysRevB.26.575610.1103/PhysRevB.26.5756 ↗
15. 10.1103/PhysRevB.16.80110.1103/PhysRevB.16.801 ↗
16. 10.1063/1.508695110.1063/1.5086951 ↗
17. 10.1038/s41467-017-01089-z10.1038/s41467-017-01089-z ↗
18. 10.1103/PhysRevB.102.20513910.1103/PhysRevB.102.205139 ↗
19. 10.1103/PhysRevB.99.24514410.1103/PhysRevB.99.245144 ↗
20. 10.1088/0305-4608/3/4/02210.1088/0305-4608/3/4/022 ↗
21. 10.1021/acsnano.0c0030310.1021/acsnano.0c00303 ↗
22. 10.1039/D0RA02499F10.1039/D0RA02499F ↗
23. 10.1103/PhysRevMaterials.1.02400510.1103/PhysRevMaterials.1.024005 ↗
24. 10.1103/PhysRevLett.117.10680110.1103/PhysRevLett.117.106801 ↗
25. 10.1021/acs.nanolett.2c0458410.1021/acs.nanolett.2c04584 ↗
26. 10.1103/PhysRevB.107.10451010.1103/PhysRevB.107.104510 ↗
27. 10.1002/qute.20180007010.1002/qute.201800070 ↗
28. 10.1103/PhysRevB.101.13450610.1103/PhysRevB.101.134506 ↗
29. 10.1107/S205225252001102110.1107/S2052252520011021 ↗
30. 10.1143/JJAP.43.L12310.1143/JJAP.43.L123 ↗
31. 10.1103/PhysRevB.50.1795310.1103/PhysRevB.50.17953 ↗
32. 10.1103/PhysRevLett.77.386510.1103/PhysRevLett.77.3865 ↗
33. 10.1016/j.scriptamat.2015.07.02110.1016/j.scriptamat.2015.07.021 ↗
34. 10.1103/PhysRevLett.107.10740310.1103/PhysRevLett.107.107403 ↗
35. 10.1016/0038-1098(81)90847-410.1016/0038-1098(81)90847-4 ↗
36. 10.1103/PhysRevB.24.420810.1103/PhysRevB.24.4208 ↗
37. 10.1002/aelm.20220045710.1002/aelm.202200457 ↗
38. 10.1021/nl200773n10.1021/nl200773n ↗
39. 10.1021/nn100393710.1021/nn1003937 ↗
40. 10.1038/srep0175510.1038/srep01755 ↗
41. 10.1038/srep0259310.1038/srep02593 ↗
42. 10.1038/s41598-020-75240-010.1038/s41598-020-75240-0 ↗
43. 10.1103/PhysRevB.107.15520310.1103/PhysRevB.107.155203 ↗
44. 10.1103/PhysRevB.92.06050210.1103/PhysRevB.92.060502 ↗
45. 10.1088/0022-3719/20/27/01110.1088/0022-3719/20/27/011 ↗
46. 10.1088/2053-1583/aa8e6c10.1088/2053-1583/aa8e6c ↗
47. 10.1021/jz301243610.1021/jz3012436 ↗
48. 10.1039/C4CS00265B10.1039/C4CS00265B ↗
49. 10.1021/acs.nanolett.6b0271010.1021/acs.nanolett.6b02710 ↗
50. 10.1021/nl303365x10.1021/nl303365x ↗
51. 10.1103/PhysRevB.105.04513410.1103/PhysRevB.105.045134 ↗