journal article·2016-08-25Open access

Tuning Optical Properties of Ge Nanocrystals by Si Shell

M. O. Nestoklon, A. N. Poddubny, P. Voisin, K. Dohnalova

The Journal of Physical Chemistry C· Volume 120· Issue 33

Abstract

We present a theoretical study of Ge-core/Si-shell nanocrystals in a wide bandgap matrix and compare the results with experimental data obtained from the samples prepared by co-sputtering. The empirical tight-binding technique allows us to account for the electronic structure under strain on the atomistic level. We find that a Si shell as thick as one monolayer is enough to reduce the radiative recombination rate as a result of valley L – X crossover. Thin Si shells lead to a dramatic reduction of the optical bandgap from the visible to the near-infrared range, which is promising for photovoltaics and photodetector applications. Our detailed analysis of the structure of the confined electron and hole states in real and reciprocal spaces indicates that the type-II heterostructure is not yet achieved for Si shells with thicknesses below 0.8 nm, despite some earlier theoretical predictions. The energy levels of holes are affected by the Si shell more than the electron states, even though holes are completely confined to the Ge core. This occurs due to a strong influence of strain on the band offsets.
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Research context

OpenAlex topics: Silicon Nanostructures and Photoluminescence · Nanowire Synthesis and Applications · Semiconductor materials and devices

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

Affiliations

Ioffe Institute, 194021 St. Petersburg, Russia

Centre de Nanosciences et de Nanotechnologies, CNRS, Université Paris-Sud, Université Paris-Saclay, 91460 Marcoussis, France

Van der Waals−Zeeman Institute, University of Amsterdam, Science Park 904, NL-1098 XH Amsterdam, The Netherlands

Funding

Stichting voor Fundamenteel Onderzoek der Materie · University of Amsterdam · Russian Science Foundation

References (66)

Show source-provided references
1. 10.1038/nphoton.2013.6710.1038/nphoton.2013.67 ↗
2. 10.1063/1.128965910.1063/1.1289659 ↗
3. 10.1063/1.175161610.1063/1.1751616 ↗
4. 10.1103/PhysRevB.76.20532110.1103/PhysRevB.76.205321 ↗
5. 10.1103/PhysRevB.77.12541410.1103/PhysRevB.77.125414 ↗
6. 10.1007/s11671-010-9688-910.1007/s11671-010-9688-9 ↗
7. 10.1021/nn102728u10.1021/nn102728u ↗
8. 10.1103/PhysRevB.51.165810.1103/PhysRevB.51.1658 ↗
9. 10.1103/PhysRevB.58.792110.1103/PhysRevB.58.7921 ↗
10. 10.1016/j.optmat.2011.07.00910.1016/j.optmat.2011.07.009 ↗
11. 10.1103/PhysRevLett.72.385110.1103/PhysRevLett.72.3851 ↗
12. 10.1007/BF0154025510.1007/BF01540255 ↗
13. 10.1063/1.36717710.1063/1.367177 ↗
14. 10.1038/ncomms566510.1038/ncomms5665 ↗
15. 10.1103/PhysRevLett.108.02740110.1103/PhysRevLett.108.027401 ↗
16. 10.1021/jz302087510.1021/jz3020875 ↗
17. 10.1021/cm503983b10.1021/cm503983b ↗
18. 10.1021/nl204089210.1021/nl2040892 ↗
19. 10.1021/nn502792m10.1021/nn502792m ↗
20. 10.1103/PhysRevB.39.187110.1103/PhysRevB.39.1871 ↗
21. 10.1063/1.353478510.1063/1.3534785 ↗
22. 10.1038/nphoton.2012.11110.1038/nphoton.2012.111 ↗
23. 10.1109/TED.2008.200688910.1109/TED.2008.2006889 ↗
24. 10.1063/1.11583810.1063/1.115838 ↗
25. 10.1063/1.12386710.1063/1.123867 ↗
26. 10.1103/PhysRevB.61.1598810.1103/PhysRevB.61.15988 ↗
27. 10.1038/ncomms191610.1038/ncomms1916 ↗
28. 10.1038/nature0583910.1038/nature05839 ↗
29. 10.1088/0957-4484/25/40/40570510.1088/0957-4484/25/40/405705 ↗
30. 10.1063/1.302706010.1063/1.3027060 ↗
31. 10.1103/PhysRevLett.91.17610110.1103/PhysRevLett.91.176101 ↗
32. 10.1063/1.200622910.1063/1.2006229 ↗
33. 10.1088/0957-4484/16/9/00710.1088/0957-4484/16/9/007 ↗
34. 10.1088/0957-4484/18/11/11571110.1088/0957-4484/18/11/115711 ↗
35. 10.1021/cm990594910.1021/cm9905949 ↗
36. 10.1021/cm202761k10.1021/cm202761k ↗
37. 10.1088/0957-4484/20/29/29560210.1088/0957-4484/20/29/295602 ↗
38. 10.1021/nn202330410.1021/nn2023304 ↗
39. 10.1016/j.matlet.2013.03.08010.1016/j.matlet.2013.03.080 ↗
40. 10.1039/C4NR06318J10.1039/C4NR06318J ↗
41. 10.1016/S0022-2313(99)00378-610.1016/S0022-2313(99)00378-6 ↗
42. 10.1103/PhysRevB.82.23540710.1103/PhysRevB.82.235407 ↗
43. 10.1063/1.143507610.1063/1.1435076 ↗
44. 10.1103/PhysRevB.72.04535110.1103/PhysRevB.72.045351 ↗
45. 10.1063/1.177288810.1063/1.1772888 ↗
46. 10.1021/jp208851610.1021/jp2088516 ↗
47. 10.1063/1.364297010.1063/1.3642970 ↗
48. 10.1039/C4CP03711A10.1039/C4CP03711A ↗
49. 10.1103/PhysRev.145.63710.1103/PhysRev.145.637 ↗
50. 10.1103/PhysRevB.52.1105910.1103/PhysRevB.52.11059 ↗
51. 10.1103/PhysRevB.57.649310.1103/PhysRevB.57.6493 ↗
52. 10.1103/PhysRevB.79.24520110.1103/PhysRevB.79.245201 ↗
53. 10.1103/PhysRevLett.84.439310.1103/PhysRevLett.84.4393 ↗
54. 10.1109/TED.2010.207115010.1109/TED.2010.2071150 ↗
55. Bricogne G. · 2006
56. 10.1103/PhysRevB.87.19542010.1103/PhysRevB.87.195420 ↗
57. 10.1103/PhysRevB.71.11521510.1103/PhysRevB.71.115215 ↗
58. 10.1088/0953-8984/19/3/03620310.1088/0953-8984/19/3/036203 ↗
59. 10.1103/PhysRevLett.104.23640310.1103/PhysRevLett.104.236403 ↗
60. 10.1103/PhysRevB.85.08520110.1103/PhysRevB.85.085201 ↗
61. Delerue C. · 200410.1007/978-3-662-08903-3 ↗
62. 10.1103/PhysRevB.47.1550010.1103/PhysRevB.47.15500 ↗
63. 10.1134/1.146916210.1134/1.1469162 ↗
64. 10.1103/PhysRevB.72.12510510.1103/PhysRevB.72.125105 ↗
65. 10.1103/PhysRevB.59.1538110.1103/PhysRevB.59.15381 ↗
66. 10.1103/PhysRevB.89.03530710.1103/PhysRevB.89.035307 ↗