journal article·2023-11-02Open access

Spin precession of light holes in the spin-orbit field of strained GaAs nanowires

D. Paget, T. Amand, H. Hijazi, A. C. H. Rowe, G. Monier, E. Gil, F. Cadiz, C. Robert Goumet, Y. André

Physical Review B· Volume 108· Issue 20

Abstract

We have used a polarized spatially resolved microluminescence technique to investigate photocarrier charge and spin transport at 6 K in a GaAs nanowire (NW; n-type doping level $\ensuremath{\approx}{10}17\phantom{\rule{0.28em}{0ex}}{\mathrm{cm}}^{\ensuremath{-}3}$). Because of the difference in expansion coefficients of the NW and of its ${\mathrm{SiO}}2$ substrate, the NW is under strain, as revealed by the splitting between light- and heavy-hole emissions in the luminescence intensity spectrum. Light valence levels lie above the heavy valence ones, which is attributed as being caused by a tensile strain along both the axial and the lateral directions of the NW, equivalent to a compressive strain in the direction of light excitation. The symmetry group of the perturbed nanowire is then lowered to ${C}2v$. No spin polarization can be evidenced for the heavy valence levels. The electron spin polarization decays up to a distance of $5\phantom{\rule{0.28em}{0ex}}\textmu{}\mathrm{m}$ from the excitation spot, because of spin relaxation, and stays constant for larger distances because of the increased value of the drift velocity. Remarkably, the light-hole spin polarization exhibits damped spatial oscillations over as much as $5\phantom{\rule{0.28em}{0ex}}\textmu{}\mathrm{m}$. Analysis of the effect of strain on valence states shows that these oscillations are caused by the spin-orbit interaction in the light valence level. It is found that, for the ${C}2v$ point group, the corresponding Hamiltonian is linear in momentum. This spin-orbit interaction causes coherent oscillations rather than a spin relaxation process since transport essentially has a drift character in the internal electric field. The equivalent effective magnetic field induced by spin-orbit interaction and strain is, taking a light-hole $g$ factor of 1, of the order of $60\phantom{\rule{0.28em}{0ex}}\mathrm{mT}$.
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Research context

OpenAlex topics: Quantum and electron transport phenomena · Semiconductor materials and devices · Nanowire Synthesis and Applications

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References (46)

Show source-provided references
1. 10.1016/j.physrep.2010.04.00210.1016/j.physrep.2010.04.002 ↗
2. 10.1103/RevModPhys.76.32310.1103/RevModPhys.76.323 ↗
3. M. I. D'yakonov · JETP Lett. · 1971 · 13 · 467
4. 10.1038/ncomms337210.1038/ncomms3372 ↗
5. 10.1126/science.117366710.1126/science.1173667 ↗
6. 10.1088/1361-6641/aa5dd610.1088/1361-6641/aa5dd6 ↗
7. 10.1038/nature0787110.1038/nature07871 ↗
8. 10.1088/1361-6641/ab315810.1088/1361-6641/ab3158 ↗
9. V. K. Kalevich · Pis'ma Zh. Eksp. Teor. Fiz. · 1990 · 52 · 230
10. 10.1038/nphys238310.1038/nphys2383 ↗
11. 10.1088/0268-1242/24/6/06400210.1088/0268-1242/24/6/064002 ↗
12. 10.1103/PhysRevLett.89.14660110.1103/PhysRevLett.89.146601 ↗
13. 10.1103/PhysRevB.46.729210.1103/PhysRevB.46.7292 ↗
14. 10.1103/PhysRevB.60.581110.1103/PhysRevB.60.5811 ↗
15. 10.1088/0268-1242/23/11/11401710.1088/0268-1242/23/11/114017 ↗
16. 10.1103/PhysRevB.89.07543010.1103/PhysRevB.89.075430 ↗
17. 10.1103/PhysRevB.85.23530810.1103/PhysRevB.85.235308 ↗
18. M. I. D'yakonov · Sov. Phys. JETP · 1986 · 63 · 655
19. 10.1063/1.11098810.1063/1.110988 ↗
20. 10.1063/1.194971810.1063/1.1949718 ↗
21. 10.1038/nature0220210.1038/nature02202 ↗
22. 10.1038/s41467-021-27006-z10.1038/s41467-021-27006-z ↗
23. 10.1103/PhysRevB.75.15330410.1103/PhysRevB.75.153304 ↗
24. 10.1103/PhysRevB.103.11541210.1103/PhysRevB.103.115412 ↗
25. 10.1021/acs.jpcc.8b0545910.1021/acs.jpcc.8b05459 ↗
26. 10.1103/PhysRevB.36.474810.1103/PhysRevB.36.4748 ↗
27. 10.1103/PhysRevB.103.19531410.1103/PhysRevB.103.195314 ↗
28. 10.1103/PhysRevB.105.19520410.1103/PhysRevB.105.195204 ↗
29. 10.1021/nl502909k10.1021/nl502909k ↗
30. 10.1063/1.349304710.1063/1.3493047 ↗
31. M. I. D'yakonov · Sov. Phys. Semicond. · 1974 · 7 · 1551
32. 10.1016/0038-1098(81)91017-610.1016/0038-1098(81)91017-6 ↗
33. A. L. Efros · 1972
34. B. I. Shklovskii · 198410.1007/978-3-662-02403-4 ↗
35. 10.1103/PhysRevB.84.07545510.1103/PhysRevB.84.075455 ↗
36. G. L. Bir · 1974
37. E. L. Ivchenko · 199710.1007/978-3-642-60650-2 ↗
38. 10.1103/PhysRevB.1.67210.1103/PhysRevB.1.672 ↗
39. 10.1103/PhysRevLett.107.13660410.1103/PhysRevLett.107.136604 ↗
40. 10.1063/1.473039610.1063/1.4730396 ↗
41. R. A. Smith · 1978
42. K. Wiesemann · 2014
43. S. Baranovskii · 2017
44. 10.1103/PhysRevB.51.1670510.1103/PhysRevB.51.16705 ↗
45. 10.1103/PhysRevB.66.24520410.1103/PhysRevB.66.245204 ↗
46. G. F. Koster · 1963