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
Source abstract
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 ↗