Observation of bright exciton splitting in strained WSe2 monolayers
Source abstract
Abstract
High-resolution magnetophotoluminescence measurements of strained ${\mathrm{WSe}}2$ monolayers are reported. At low temperature, a splitting of a few meV in the neutral exciton peak is observed, which is attributed to the theoretically predicted in-plane ($xy$) anisotropy splitting. Measurements in high magnetic fields up to 30 T demonstrate that strain and intervalley electron-hole exchange mix the valley-exciton energy levels, leading to a relaxation of the valley-selective optical selection rules and to strongly modified exciton $g$ factors. Our observation of the bright exciton splitting provides crucial information about the dispersion of valley excitons and paves the way to develop valley functionality for photonic devices.
Source: openalex_inverted_index · Quality: baseline
Research context
OpenAlex topics: 2D Materials and Applications · Perovskite Materials and Applications · Strong Light-Matter Interactions
SciVX discovery tags are terminology-based. OpenAlex topics are source-provided classifications.
References (44)
Show source-provided references
1. 10.1038/nphys294210.1038/nphys2942 ↗
2. 10.1038/nphoton.2015.28210.1038/nphoton.2015.282 ↗
3. 10.1038/natrevmats.2016.5510.1038/natrevmats.2016.55 ↗
4. 10.1093/nsr/nwu07810.1093/nsr/nwu078 ↗
5. 10.1515/nanoph-2016-016510.1515/nanoph-2016-0165 ↗
6. 10.1038/nmat350510.1038/nmat3505 ↗
7. 10.1038/ncomms188210.1038/ncomms1882 ↗
8. 10.1038/nnano.2013.15110.1038/nnano.2013.151 ↗
9. 10.1038/nphys320310.1038/nphys3203 ↗
10. 10.1038/nphys320110.1038/nphys3201 ↗
11. 10.1021/acs.nanolett.5b0062610.1021/acs.nanolett.5b00626 ↗
12. 10.1088/2053-1583/2/3/03400210.1088/2053-1583/2/3/034002 ↗
13. 10.1103/PhysRevB.93.16541210.1103/PhysRevB.93.165412 ↗
14. 10.1103/PhysRevB.41.753610.1103/PhysRevB.41.7536 ↗
15. 10.1103/PhysRevB.47.1577610.1103/PhysRevB.47.15776 ↗
16. 10.1103/PhysRevB.65.19531510.1103/PhysRevB.65.195315 ↗
17. 10.1038/ncomms128110.1038/ncomms1281 ↗
18. 10.1103/PhysRevB.89.20130210.1103/PhysRevB.89.201302 ↗
19. 10.1038/ncomms1271510.1038/ncomms12715 ↗
20. 10.1038/nphys360410.1038/nphys3604 ↗
21. 10.1002/pssb.20155221110.1002/pssb.201552211 ↗
22. 10.1073/pnas.161012311410.1073/pnas.1610123114 ↗
23. 10.1103/PhysRevB.81.12531110.1103/PhysRevB.81.125311 ↗
24. 10.1016/j.ssc.2006.07.01610.1016/j.ssc.2006.07.016 ↗
25. 10.1038/ncomms487610.1038/ncomms4876 ↗
26. 10.1021/acs.nanolett.5b0009210.1021/acs.nanolett.5b00092 ↗
27. 10.1039/C4CS00282B10.1039/C4CS00282B ↗
28. 10.1103/PhysRevB.87.16540910.1103/PhysRevB.87.165409 ↗
29. 10.1021/acs.nanolett.6b0494410.1021/acs.nanolett.6b04944 ↗
30. 10.1103/PhysRev.137.A178410.1103/PhysRev.137.A1784 ↗
31. 10.1103/PhysRevB.91.12140910.1103/PhysRevB.91.121409 ↗
32. 10.1021/acs.nanolett.7b0486810.1021/acs.nanolett.7b04868 ↗
33. 10.1103/PhysRevLett.108.19680210.1103/PhysRevLett.108.196802 ↗
34. 10.1103/PhysRevB.86.24140110.1103/PhysRevB.86.241401 ↗
35. 10.1073/pnas.050284810210.1073/pnas.0502848102 ↗
36. 10.1103/PhysRevB.90.07541310.1103/PhysRevB.90.075413 ↗
37. 10.1103/PhysRevX.6.02102410.1103/PhysRevX.6.021024 ↗
38. 10.1103/PhysRevB.72.23530610.1103/PhysRevB.72.235306 ↗
39. 10.1021/nn501026t10.1021/nn501026t ↗
40. 10.1103/PhysRevLett.79.397410.1103/PhysRevLett.79.3974 ↗
41. 10.1103/PhysRevB.96.04130210.1103/PhysRevB.96.041302 ↗
42. 10.1103/PhysRevLett.113.26680410.1103/PhysRevLett.113.266804 ↗
43. 10.1103/PhysRevLett.114.03740110.1103/PhysRevLett.114.037401 ↗
44. 10.1103/PhysRevB.92.19540210.1103/PhysRevB.92.195402 ↗