journal article·2021-09Open access

Heterogeneities and Emissive Defects in MAPbI3 Perovskite Revealed by Spectrally Resolved Luminescence Blinking

Marina Gerhard, Boris Louis, Pavel A. Frantsuzov, Jun Li, Alexander Kiligaridis, Johan Hofkens, Ivan G. Scheblykin

Advanced Optical Materials· Volume 9· Issue 18

Abstract

Abstract The fate of excited charge carriers in metal halide perovskite semiconductors is influenced by energetic disorder and defects. Here, photoluminescence (PL) blinking is used to probe metastable nonradiative (NR) centers and the nanoscale energy landscape. Temporal activation of an NR center creates a local region with increased NR recombination. Activation and deactivation of this local PL quenching does not only lead to PL blinking, but also to fluctuations of the PL spectra, if the crystal is inhomogeneous in the sense that the PL emission spectrum is slightly different from one location to another. It resembles the spectral hole‐burning technique; however, here the eliminated excited states are chosen by their spatial localization close to the quencher. In MAPbI3, PL spectral fluctuations at low temperature reveal energetic inhomogeneities on the order of 5 to 10 meV. Quenching of the main PL band is often found to correlate with an increase of the low‐energetic tail of the PL spectra, which is attributed to partially radiative recombination of charges captured by the NR center. The transition energy of the NR center is found to be only ≈80 meV smaller than the bandgap, implying that the underlying defect cannot be a single mid‐bandgap state.
Source: crossref · Quality: baseline

Research context

OpenAlex topics: Perovskite Materials and Applications · Quantum Dots Synthesis And Properties · Chalcogenide Semiconductor Thin Films

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

Affiliations

Faculty of Physics and Materials Sciences Center Renthof 7a Marburg 35032 Germany

Division of Chemical Physics and NanoLund Lund University Box 124 Lund 22100 Sweden

Molecular Imaging and Photonics Celestijnenlaan 200F Box 2404 Leuven 3001 Belgium

Voevodsky Institute of Chemical Kinetics and Combustion SB RAS Institutskaya str. 3 Novosibirsk 630090 Russia

Institute of Spectroscopy RAS Moscow 108840 Russia

Funding

Vetenskapsrådet · Knut och Alice Wallenbergs Stiftelse · China Scholarship Council · Russian Science Foundation

References (63)

Show source-provided references
1. 10.1038/natrevmats.2015.710.1038/natrevmats.2015.7 ↗
2. 10.1038/nnano.2015.9010.1038/nnano.2015.90 ↗
3. National Renewable Energy Laboratory https://www.nrel.gov/pv/assets/pdfs/best‐research‐cell‐efficiencies.20200708.pdf(accessed: December 2020).
4. 10.1021/jz500528510.1021/jz5005285 ↗
5. 10.1038/nmat391110.1038/nmat3911 ↗
6. 10.1038/nenergy.2016.14910.1038/nenergy.2016.149 ↗
7. 10.1021/acsenergylett.7b0023910.1021/acsenergylett.7b00239 ↗
8. 10.1039/C9MH00500E10.1039/C9MH00500E ↗
9. 10.1002/adma.20150229410.1002/adma.201502294 ↗
10. 10.1021/acsenergylett.7b0054710.1021/acsenergylett.7b00547 ↗
11. 10.1063/1.486477810.1063/1.4864778 ↗
12. 10.1021/nl502612m10.1021/nl502612m ↗
13. 10.1002/adfm.20140442110.1002/adfm.201404421 ↗
14. 10.1021/jz500858a10.1021/jz500858a ↗
15. 10.1038/s41467-017-00058-w10.1038/s41467-017-00058-w ↗
16. 10.1103/PhysRevApplied.2.03400710.1103/PhysRevApplied.2.034007 ↗
17. 10.1126/science.aaa533310.1126/science.aaa5333 ↗
18. 10.1021/acsnano.6b0740710.1021/acsnano.6b07407 ↗
19. 10.1021/acsnano.7b0624210.1021/acsnano.7b06242 ↗
20. 10.1021/nl504139710.1021/nl5041397 ↗
21. 10.1021/acsomega.6b0010710.1021/acsomega.6b00107 ↗
22. 10.1002/anie.20180485210.1002/anie.201804852 ↗
23. 10.1038/ncomms1089610.1038/ncomms10896 ↗
24. 10.1002/adfm.20170086010.1002/adfm.201700860 ↗
25. 10.1126/sciadv.160115610.1126/sciadv.1601156 ↗
26. 10.1038/s41467-019-08326-710.1038/s41467-019-08326-7 ↗
27. 10.1063/1.205819210.1063/1.2058192 ↗
28. 10.1093/acprof:oso/9780199588336.001.000110.1093/acprof:oso/9780199588336.001.0001 ↗
29. 10.1063/1.45346710.1063/1.453467 ↗
30. 10.1063/1.489159510.1063/1.4891595 ↗
31. 10.1002/adfm.20150234010.1002/adfm.201502340 ↗
32. 10.1021/acs.jpclett.6b0078110.1021/acs.jpclett.6b00781 ↗
33. 10.1039/C5CP02605A10.1039/C5CP02605A ↗
34. 10.1038/ncomms1133010.1038/ncomms11330 ↗
35. 10.1039/C4CP03573A10.1039/C4CP03573A ↗
36. 10.1021/acs.nanolett.5b0140510.1021/acs.nanolett.5b01405 ↗
37. 10.1002/adma.20170549410.1002/adma.201705494 ↗
38. 10.1038/s41467-019-09640-w10.1038/s41467-019-09640-w ↗
39. 10.1366/12-0665510.1366/12-06655 ↗
40. 10.1146/annurev.pc.40.100189.00243510.1146/annurev.pc.40.100189.002435 ↗
41. 10.1021/acs.jpcc.8b0386210.1021/acs.jpcc.8b03862 ↗
42. 10.7326/0003-4819-130-12-199906150-0000810.7326/0003-4819-130-12-199906150-00008 ↗
43. 10.1038/349225a010.1038/349225a0 ↗
44. 10.1002/cphc.20100067810.1002/cphc.201000678 ↗
45. 10.1063/1.476632110.1063/1.4766321 ↗
46. 10.1126/science.278.5346.211410.1126/science.278.5346.2114 ↗
47. 10.1103/PhysRevLett.85.330110.1103/PhysRevLett.85.3301 ↗
48. 10.1103/PhysRevLett.86.488310.1103/PhysRevLett.86.4883 ↗
49. 10.1063/1.512491310.1063/1.5124913 ↗
50. 10.1103/PhysRevLett.103.20740210.1103/PhysRevLett.103.207402 ↗
51. 10.1021/acs.jpclett.6b0226110.1021/acs.jpclett.6b02261 ↗
52. 10.1039/C7EE03543H10.1039/C7EE03543H ↗
53. 10.1021/acs.jpclett.9b0387810.1021/acs.jpclett.9b03878 ↗
54. 10.1021/acs.jpclett.6b0120710.1021/acs.jpclett.6b01207 ↗
55. 10.1038/ncomms1175510.1038/ncomms11755 ↗
56. 10.1002/pssb.222153022210.1002/pssb.2221530222 ↗
57. 10.1063/1.275592710.1063/1.2755927 ↗
58. 10.1103/PhysRevB.72.15532110.1103/PhysRevB.72.155321 ↗
59. 10.1103/PhysRevB.15.98910.1103/PhysRevB.15.989 ↗
60. 10.1038/ncomms849710.1038/ncomms8497 ↗
61. 10.1039/C5EE01265A10.1039/C5EE01265A ↗
62. 10.1021/jacs.9b1239110.1021/jacs.9b12391 ↗
63. 10.1063/1.142741710.1063/1.1427417 ↗