journal article·2017-04-25

Optimizing Charge Injection across Transition Metal Dichalcogenide Heterojunctions: Theory and Experiment

Jie Guan, Hsun-Jen Chuang, Zhixian Zhou, David Tománek

ACS Nano· Volume 11· Issue 4
Publisher page

Abstract

In search of an improved strategy to form low-resistance contacts to semiconducting transition metal dichalcogenides, we combine ab initio density functional electronic structure calculations for an NbSe 2 /WSe 2 interface with quantum transport measurements of the corresponding heterojunction between a few-layer WSe 2 semiconductor and a metallic NbSe 2 layer. Our theoretical results suggest that, besides a rigid band shift associated with charge transfer, the presence of NbSe 2 does not modify the electronic structure of WSe 2 . Since the two transition metal dichalcogenides are structurally similar and display only a small lattice mismatch, their heterojunction can efficiently transfer charge across the interface. These findings are supported by transport measurements for WSe 2 field-effect transistors with NbSe 2 contacts, which exhibit nearly ohmic behavior and phonon-limited mobility in the hole channel, indicating that the contacts to WSe 2 are highly transparent.
Source: openalex_inverted_index · Quality: baseline

Research context

OpenAlex topics: 2D Materials and Applications · MXene and MAX Phase Materials · Graphene research and applications

SciVX discovery tags are terminology-based. OpenAlex topics are source-provided classifications.

Affiliations

Physics and Astronomy Department, Michigan State University, East Lansing, Michigan 48824, United States

Physics and Astronomy Department, Wayne State University, Detroit, Michigan 48201, United States

Funding

Division of Emerging Frontiers in Research and Innovation · Air Force Office of Scientific Research · Wayne State University · Division of Materials Research

References (57)

Show source-provided references
1. 10.1103/PhysRevLett.28.29910.1103/PhysRevLett.28.299 ↗
2. 10.1073/pnas.050284810210.1073/pnas.0502848102 ↗
3. 10.1103/PhysRevLett.105.13680510.1103/PhysRevLett.105.136805 ↗
4. 10.1038/nnano.2010.27910.1038/nnano.2010.279 ↗
5. 10.1038/nnano.2012.19310.1038/nnano.2012.193 ↗
6. 10.1021/nn500064s10.1021/nn500064s ↗
7. 10.1063/1.482040810.1063/1.4820408 ↗
8. 10.1021/nn303513c10.1021/nn303513c ↗
9. 10.1021/nl303583v10.1021/nl303583v ↗
10. 10.1063/1.476821810.1063/1.4768218 ↗
11. 10.1021/nl400044m10.1021/nl400044m ↗
12. 10.1109/LED.2013.227731110.1109/LED.2013.2277311 ↗
13. 10.1021/ja503332710.1021/ja5033327 ↗
14. 10.1021/nl502603d10.1021/nl502603d ↗
15. 10.1021/nl503251h10.1021/nl503251h ↗
16. 10.1002/adma.20160110410.1002/adma.201601104 ↗
17. 10.1103/PhysRevLett.108.15680210.1103/PhysRevLett.108.156802 ↗
18. 10.1088/0953-8984/27/13/13320310.1088/0953-8984/27/13/133203 ↗
19. 10.1038/srep2178610.1038/srep21786 ↗
20. 10.1039/C5NR06204G10.1039/C5NR06204G ↗
21. 10.1103/PhysRevX.4.03100510.1103/PhysRevX.4.031005 ↗
22. 10.1021/nl303909f10.1021/nl303909f ↗
23. 10.1021/nl403465v10.1021/nl403465v ↗
24. 10.1021/acsnano.5b0461110.1021/acsnano.5b04611 ↗
25. 10.1088/2053-1583/3/2/02100710.1088/2053-1583/3/2/021007 ↗
26. 10.1038/nmat408010.1038/nmat4080 ↗
27. 10.1126/science.aab317510.1126/science.aab3175 ↗
28. 10.1126/sciadv.160006910.1126/sciadv.1600069 ↗
29. 10.1021/nl501275p10.1021/nl501275p ↗
30. 10.1109/LED.2014.231334010.1109/LED.2014.2313340 ↗
31. 10.1021/nl504957p10.1021/nl504957p ↗
32. 10.1021/nl901572a10.1021/nl901572a ↗
33. 10.1021/acs.nanolett.5b0506610.1021/acs.nanolett.5b05066 ↗
34. 10.1103/PhysRevB.91.16130410.1103/PhysRevB.91.161304 ↗
35. 10.1021/nl500903710.1021/nl5009037 ↗
36. 10.1021/nn501723y10.1021/nn501723y ↗
37. 10.1038/nnano.2015.7010.1038/nnano.2015.70 ↗
38. 10.1016/0022-4596(72)90158-210.1016/0022-4596(72)90158-2 ↗
39. 10.1016/0022-4596(87)90057-010.1016/0022-4596(87)90057-0 ↗
40. 10.1016/j.commatsci.2005.04.01010.1016/j.commatsci.2005.04.010 ↗
41. 10.1002/jcc.2057510.1002/jcc.20575 ↗
42. 10.1088/0953-8984/21/8/08420410.1088/0953-8984/21/8/084204 ↗
43. 10.1063/1.355371610.1063/1.3553716 ↗
44. 10.1021/nn402954e10.1021/nn402954e ↗
45. 10.1021/nn401053g10.1021/nn401053g ↗
46. 10.1038/nmat368710.1038/nmat3687 ↗
47. 10.1021/nn501150r10.1021/nn501150r ↗
48. 10.1039/c3dt51903a10.1039/c3dt51903a ↗
49. Sata Y. · Condensed Matter · 2017 · 1
50. 10.1103/PhysRevB.54.1116910.1103/PhysRevB.54.11169 ↗
51. 10.1103/PhysRevB.47.55810.1103/PhysRevB.47.558 ↗
52. 10.1103/PhysRevB.49.1425110.1103/PhysRevB.49.14251 ↗
53. 10.1103/PhysRevB.59.175810.1103/PhysRevB.59.1758 ↗
54. 10.1088/0953-8984/22/2/02220110.1088/0953-8984/22/2/022201 ↗
55. 10.1103/PhysRevB.83.19513110.1103/PhysRevB.83.195131 ↗
56. 10.1103/PhysRevB.13.518810.1103/PhysRevB.13.5188 ↗
57. 10.6028/jres.049.04410.6028/jres.049.044 ↗