journal article·2019-12-12Open access

Layer and orbital interference effects in photoemission from transition metal dichalcogenides

Habib Rostami, Klara Volckaert, Nicola Lanata, Sanjoy K. Mahatha, Charlotte E. Sanders, Marco Bianchi, Daniel Lizzit, Luca Bignardi, Silvano Lizzit, Jill A. Miwa, Alexander V. Balatsky, Philip Hofmann, Søren Ulstrup

Physical Review B· Volume 100· Issue 23

Abstract

In this work, we provide an effective model to evaluate the one-electron dipole matrix elements governing optical excitations and the photoemission process of single-layer (SL) and bilayer (BL) transition metal dichalcogenides. By utilizing a $\mathbit{k}\ifmmode\cdot\else\textperiodcentered\fi{}\mathbit{p}$ Hamiltonian, we calculate the photoemission intensity as observed in angle-resolved photoemission from the valence bands around the $\overline{K}$ valley of ${\mathrm{MoS}}2$. In SL ${\mathrm{MoS}}2$, we find a significant masking of intensity outside the first Brillouin zone, which originates from an in-plane interference effect between photoelectrons emitted from the Mo $d$ orbitals. In BL ${\mathrm{MoS}}2$, an additional interlayer interference effect leads to a distinctive modulation of intensity with photon energy. Finally, we use the semiconductor Bloch equations to model the optical excitation in a time- and angle-resolved pump-probe photoemission experiment. We find that the momentum dependence of an optically excited population in the conduction band leads to an observable dichroism in both SL and BL ${\mathrm{MoS}}2$.
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OpenAlex topics: 2D Materials and Applications · Ga2O3 and related materials · Graphene research and applications

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References (59)

Show source-provided references
1. 10.1103/PhysRevLett.108.19680210.1103/PhysRevLett.108.196802 ↗
2. 10.1038/nnano.2012.9510.1038/nnano.2012.95 ↗
3. 10.1038/nnano.2012.9610.1038/nnano.2012.96 ↗
4. 10.1038/ncomms188210.1038/ncomms1882 ↗
5. 10.1038/nphys320310.1038/nphys3203 ↗
6. 10.1038/nphys320110.1038/nphys3201 ↗
7. 10.1103/PhysRevB.87.16140310.1103/PhysRevB.87.161403 ↗
8. 10.1038/nphys269110.1038/nphys2691 ↗
9. 10.1038/ncomms305310.1038/ncomms3053 ↗
10. 10.1038/nphys284810.1038/nphys2848 ↗
11. 10.1038/nphys310510.1038/nphys3105 ↗
12. 10.1038/nnano.2015.21710.1038/nnano.2015.217 ↗
13. 10.1103/PhysRevLett.118.08640210.1103/PhysRevLett.118.086402 ↗
14. 10.1088/2053-1583/2/2/02200110.1088/2053-1583/2/2/022001 ↗
15. 10.1103/PhysRevB.88.04541610.1103/PhysRevB.88.045416 ↗
16. 10.1103/PhysRevB.88.08544010.1103/PhysRevB.88.085440 ↗
17. 10.1103/PhysRevLett.114.04680210.1103/PhysRevLett.114.046802 ↗
18. 10.1103/PhysRevB.100.24140610.1103/PhysRevB.100.241406 ↗
19. S. Hüfner · 200310.1007/978-3-662-09280-4 ↗
20. 10.1103/PhysRevB.51.1361410.1103/PhysRevB.51.13614 ↗
21. 10.1103/PhysRevB.77.19540310.1103/PhysRevB.77.195403 ↗
22. 10.1038/nphys161510.1038/nphys1615 ↗
23. 10.1103/PhysRevB.83.12140810.1103/PhysRevB.83.121408 ↗
24. 10.1103/PhysRevLett.107.16680310.1103/PhysRevLett.107.166803 ↗
25. 10.1021/nl300512q10.1021/nl300512q ↗
26. 10.1103/PhysRevLett.107.20760210.1103/PhysRevLett.107.207602 ↗
27. 10.1103/PhysRevB.84.24543510.1103/PhysRevB.84.245435 ↗
28. 10.1103/PhysRevLett.108.04680510.1103/PhysRevLett.108.046805 ↗
29. 10.1103/PhysRevLett.107.07760110.1103/PhysRevLett.107.077601 ↗
30. 10.1103/PhysRevLett.110.21640110.1103/PhysRevLett.110.216401 ↗
31. 10.1103/PhysRevLett.110.21680110.1103/PhysRevLett.110.216801 ↗
32. 10.1103/PhysRevLett.112.07680210.1103/PhysRevLett.112.076802 ↗
33. 10.1103/PhysRevLett.115.01680110.1103/PhysRevLett.115.016801 ↗
34. 10.1016/j.nima.2004.01.03910.1016/j.nima.2004.01.039 ↗
35. 10.1021/acs.nanolett.5b0196710.1021/acs.nanolett.5b01967 ↗
36. 10.1103/PhysRevB.94.20540610.1103/PhysRevB.94.205406 ↗
37. 10.1103/PhysRevLett.117.27720110.1103/PhysRevLett.117.277201 ↗
38. 10.1103/PhysRevB.95.04140510.1103/PhysRevB.95.041405 ↗
39. 10.1103/PhysRevLett.123.23680210.1103/PhysRevLett.123.236802 ↗
40. 10.1103/RevModPhys.75.47310.1103/RevModPhys.75.473 ↗
41. 10.1038/s41535-019-0194-810.1038/s41535-019-0194-8 ↗
42. 10.1088/0034-4885/59/10/00210.1088/0034-4885/59/10/002 ↗
43. 10.1016/j.elspec.2016.11.00710.1016/j.elspec.2016.11.007 ↗
44. 10.1016/j.ultramic.2016.07.01610.1016/j.ultramic.2016.07.016 ↗
45. 10.1038/nphys252410.1038/nphys2524 ↗
46. 10.1103/PhysRev.34.10910.1103/PhysRev.34.109 ↗
47. 10.1088/0953-8984/28/49/49500110.1088/0953-8984/28/49/495001 ↗
48. 10.1103/PhysRevB.86.24140110.1103/PhysRevB.86.241401 ↗
49. 10.1103/PhysRevB.85.20530210.1103/PhysRevB.85.205302 ↗
50. 10.1103/PhysRevB.92.19540210.1103/PhysRevB.92.195402 ↗
51. 10.1103/PhysRevB.98.03540810.1103/PhysRevB.98.035408 ↗
52. 10.1103/PhysRevB.64.23530510.1103/PhysRevB.64.235305 ↗
53. 10.1103/PhysRevB.99.16542110.1103/PhysRevB.99.165421 ↗
54. 10.1021/acsnano.6b0262210.1021/acsnano.6b02622 ↗
55. 10.1103/PhysRevLett.111.02740310.1103/PhysRevLett.111.027403 ↗
56. H. Haug · 199410.1142/2451 ↗
57. F. Rossi · 2010
58. 10.1103/PhysRevB.53.701010.1103/PhysRevB.53.7010 ↗
59. 10.1103/PhysRevB.77.23540610.1103/PhysRevB.77.235406 ↗