journal article·2025-03-26

Magnetic field induced circular polarization of the exciton luminescence of (In,Al)As/AlAs quantum dots with indirect band gap and type-I band alignment

Lyubov V. Kotova, Timur S. Shamirzaev, Dmitri R. Yakovlev, Vladimir P. Kochereshko, Manfred Bayer

Physical Review B· Volume 111· Issue 11
Publisher page

Abstract

The circularly polarized photoluminescence (PL) of excitons induced by application of a magnetic field is investigated experimentally and theoretically for an inhomogeneous ensemble of (In,Al)As/AlAs quantum dots with indirect band gap and type-I band alignment. We demonstrate that the circular polarization degree of the PL shows a nonmonotonic dependence on the dot size and the splitting of the oppositely polarized emission bands is significantly larger than the Zeeman splitting of the excitons in individual dots. The low-energy polarized luminescence band has lower intensity than the high-energy one. The polarization sign of the exciton emission coincides in large dots and the wetting layer, while it is opposite in small dots. A model description of this phenomenon that takes into account the equilibrium populations of long-lived exciton states is developed. The dependence of the exciton $g$ factor on the size of the quantum dot is obtained. Good agreement of the modeled spectra with the experimentally observed ones is achieved without any fitting parameters.
Source: openalex_inverted_index · Quality: baseline

Research context

OpenAlex topics: Semiconductor Quantum Structures and Devices · Quantum Dots Synthesis And Properties · Quantum and electron transport phenomena

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

Affiliations

Ioffe Institute

Russian Academy of Sciences

Institute of Semiconductor Physics

Technische Universität Dortmund

Funding

Russian Science Foundation

References (49)

Show source-provided references
1. 2016
2. 10.1038/nphoton.2016.2310.1038/nphoton.2016.23 ↗
3. 10.1016/j.physrep.2010.04.00210.1016/j.physrep.2010.04.002 ↗
4. 10.1103/PhysRevLett.125.15680110.1103/PhysRevLett.125.156801 ↗
5. 10.1103/RevModPhys.80.151710.1103/RevModPhys.80.1517 ↗
6. 10.1103/PhysRevB.61.1263910.1103/PhysRevB.61.12639 ↗
7. 10.1134/S106378341808012710.1134/S1063783418080127 ↗
8. 10.1134/S106378341808022X10.1134/S106378341808022X ↗
9. 10.1103/PhysRevB.83.23531710.1103/PhysRevB.83.235317 ↗
10. 10.1063/1.291781110.1063/1.2917811 ↗
11. 10.1103/PhysRevB.78.08532310.1103/PhysRevB.78.085323 ↗
12. 10.1103/PhysRevB.84.15531810.1103/PhysRevB.84.155318 ↗
13. 10.1103/PhysRevB.90.12543110.1103/PhysRevB.90.125431 ↗
14. 10.1103/PhysRevB.75.24530210.1103/PhysRevB.75.245302 ↗
15. 2005
16. 10.1103/PhysRevB.97.24530610.1103/PhysRevB.97.245306 ↗
17. 10.1103/PhysRevB.104.19530610.1103/PhysRevB.104.195306 ↗
18. 10.1103/PhysRevB.104.04530510.1103/PhysRevB.104.045305 ↗
19. 10.1063/1.353210210.1063/1.3532102 ↗
20. 10.1088/0268-1242/21/4/01910.1088/0268-1242/21/4/019 ↗
21. 10.1063/1.204254310.1063/1.2042543 ↗
22. 10.1103/PhysRevB.99.19541110.1103/PhysRevB.99.195411 ↗
23. 10.1103/PhysRevB.65.03531310.1103/PhysRevB.65.035313 ↗
24. 10.1103/PhysRevB.94.04541110.1103/PhysRevB.94.045411 ↗
25. 10.1103/PhysRevB.96.03530210.1103/PhysRevB.96.035302 ↗
26. 10.1103/PhysRevB.76.15530910.1103/PhysRevB.76.155309 ↗
27. 10.1103/PhysRevB.78.08520410.1103/PhysRevB.78.085204 ↗
28. 10.1103/PhysRevB.55.1570110.1103/PhysRevB.55.15701 ↗
29. 10.1103/PhysRevB.50.888910.1103/PhysRevB.50.8889 ↗
30. 10.1103/PhysRevB.104.20542310.1103/PhysRevB.104.205423 ↗
31. 1988
32. 10.1134/S106378261506021410.1134/S1063782615060214 ↗
33. 10.1002/pssc.20100084710.1002/pssc.201000847 ↗
34. 10.1103/PhysRev.124.65710.1103/PhysRev.124.657 ↗
35. 10.1119/1.197193110.1119/1.1971931 ↗
36. L. Landau · 1958
37. 10.1103/PhysRevB.3.43910.1103/PhysRevB.3.439 ↗
38. 10.1002/pssb.20098318810.1002/pssb.200983188 ↗
39. 10.1103/PhysRevLett.83.354610.1103/PhysRevLett.83.3546 ↗
40. 10.1103/PhysRevB.107.23530210.1103/PhysRevB.107.235302 ↗
41. 2000
42. E. Ivchenko · 199710.1007/978-3-642-60650-2 ↗
43. 10.1063/1.497535310.1063/1.4975353 ↗
44. 10.1063/1.486864410.1063/1.4868644 ↗
45. 10.1063/1.224521310.1063/1.2245213 ↗
46. 10.1063/1.480830210.1063/1.4808302 ↗
47. 10.1016/j.physe.2011.12.00310.1016/j.physe.2011.12.003 ↗
48. 10.1103/PhysRevB.102.12541210.1103/PhysRevB.102.125412 ↗
49. 10.1103/PhysRevB.93.20542510.1103/PhysRevB.93.205425 ↗