Momentum-resolved linear dichroism in bilayerMoS2
Source abstract
Abstract
In solid state photoemission experiments it is possible to extract information about the symmetry and orbital character of the electronic wave functions via the photoemission selection rules that shape the measured intensity. This approach can be expanded in a pump-probe experiment where the intensity contains additional information about interband excitations induced by an ultrafast laser pulse with tunable polarization. Here, we find an unexpected strong linear dichroism effect (up to 42.4%) in the conduction band of bilayer ${\mathrm{MoS}}2$, when measuring energy- and momentum-resolved snapshots of excited electrons by time- and angle-resolved photoemission spectroscopy. We model the polarization-dependent photoemission intensity in the transiently populated conduction band using the semiconductor Bloch equations. Our theoretical analysis reveals a strongly anisotropic momentum dependence of the optical excitations due to intralayer single-particle hopping, which explains the observed linear dichroism.
Source: openalex_inverted_index · Quality: baseline
Research context
OpenAlex topics: 2D Materials and Applications · Perovskite Materials and Applications · MXene and MAX Phase Materials
SciVX discovery tags are terminology-based. OpenAlex topics are source-provided classifications.
References (43)
Show source-provided references
1. B. Henderson · 200610.1093/oso/9780199298624.001.0001 ↗
2. 10.1103/PhysRevB.21.324510.1103/PhysRevB.21.3245 ↗
3. 10.1021/nl300512q10.1021/nl300512q ↗
4. 10.1103/PhysRevLett.110.21640110.1103/PhysRevLett.110.216401 ↗
5. 10.1038/nphys268510.1038/nphys2685 ↗
6. 10.1103/PhysRevLett.121.18640110.1103/PhysRevLett.121.186401 ↗
7. 10.1103/PhysRevLett.108.19680210.1103/PhysRevLett.108.196802 ↗
8. 10.1126/science.125014010.1126/science.1250140 ↗
9. 10.1038/nnano.2012.9610.1038/nnano.2012.96 ↗
10. 10.1038/nnano.2012.9510.1038/nnano.2012.95 ↗
11. 10.1103/PhysRevLett.99.19700110.1103/PhysRevLett.99.197001 ↗
12. 10.1103/PhysRevB.84.20540610.1103/PhysRevB.84.205406 ↗
13. 10.1038/nature0982910.1038/nature09829 ↗
14. 10.1103/PhysRevLett.111.02740310.1103/PhysRevLett.111.027403 ↗
15. 10.1021/acs.nanolett.5b0196710.1021/acs.nanolett.5b01967 ↗
16. 10.1103/PhysRevLett.117.27720110.1103/PhysRevLett.117.277201 ↗
17. 10.1103/PhysRevB.96.02030110.1103/PhysRevB.96.020301 ↗
18. 10.1103/PhysRevB.95.04140510.1103/PhysRevB.95.041405 ↗
19. 10.1103/PhysRevLett.123.23680210.1103/PhysRevLett.123.236802 ↗
20. 10.1103/PhysRevB.96.23544010.1103/PhysRevB.96.235440 ↗
21. 10.1016/S0167-5729(03)00013-X10.1016/S0167-5729(03)00013-X ↗
22. 10.1016/S0169-4332(99)00253-610.1016/S0169-4332(99)00253-6 ↗
23. 10.1103/PhysRevB.63.07540410.1103/PhysRevB.63.075404 ↗
24. 10.1021/acs.langmuir.5b0253310.1021/acs.langmuir.5b02533 ↗
25. 10.1103/PhysRevB.92.24544210.1103/PhysRevB.92.245442 ↗
26. 10.1088/2053-1583/aabb7410.1088/2053-1583/aabb74 ↗
27. 10.1016/j.surfrep.2006.10.00110.1016/j.surfrep.2006.10.001 ↗
28. 10.1088/0022-3719/13/5/02410.1088/0022-3719/13/5/024 ↗
29. 10.1103/PhysRevB.89.07540910.1103/PhysRevB.89.075409 ↗
30. 10.1016/j.nima.2004.01.03910.1016/j.nima.2004.01.039 ↗
31. 10.1088/0953-8984/27/16/16420610.1088/0953-8984/27/16/164206 ↗
32. 10.1103/PhysRevB.100.23542310.1103/PhysRevB.100.235423 ↗
33. 10.1016/j.elspec.2016.11.00710.1016/j.elspec.2016.11.007 ↗
34. 10.1103/PhysRevB.88.04541610.1103/PhysRevB.88.045416 ↗
35. 10.1103/PhysRevB.88.08544010.1103/PhysRevB.88.085440 ↗
36. 10.1088/0953-8984/28/49/49500110.1088/0953-8984/28/49/495001 ↗
37. 10.1038/ncomms305310.1038/ncomms3053 ↗
38. 10.1103/PhysRevB.98.03540810.1103/PhysRevB.98.035408 ↗
39. H. Haug · 200410.1142/5394 ↗
40. 10.1038/nphys310510.1038/nphys3105 ↗
41. 10.1103/PhysRevLett.114.04680210.1103/PhysRevLett.114.046802 ↗
42. 10.1103/PhysRevLett.121.13640210.1103/PhysRevLett.121.136402 ↗
43. 10.17630/401b4d4d-406f-47b6-bb0f- 45b0df94903d10.17630/401b4d4d-406f-47b6-bb0f- 45b0df94903d ↗