journal article·2024-01-09Open access

Hot Excitons Cool in Metal Halide Perovskite Nanocrystals as Fast as CdSe Nanocrystals

Dallas P. Strandell, Davide Zenatti, Priya Nagpal, Arnab Ghosh, Dmitry N. Dirin, Maksym V. Kovalenko, Patanjali Kambhampati

ACS Nano· Volume 18· Issue 1

Abstract

The idea of phonon bottlenecks has long been pursued in nanoscale materials for their application in hot exciton devices, such as photovoltaics. Decades ago, it was shown that there is no quantum phonon bottleneck in strongly confined quantum dots due to their physics of quantum confinement. More recently, it was proposed that there are hot phonon bottlenecks in metal halide perovskites due to their physics. Recent work has called into question these bottlenecks in metal halide perovskites. Here, we compare hot exciton cooling in a range of sizes of CsPbBr 3 nanocrystals from weakly to strongly confined. These results are compared to strongly confined CdSe quantum dots of two sizes and degrees of quantum confinement. CdSe is a model system as a ruler for measuring hot exciton cooling being fast, by virtue of its efficient Auger-assisted processes. By virtue of 3 ps time resolution, the hot exciton photoluminescence can now be directly observed, which is the most direct measure of the presence of hot excitons and their lifetimes. The hot exciton photoluminescence decays on nearly the same 2 ps time scale on both the weakly confined perovskite and the larger CdSe quantum dots, much faster than the 10 ps cooling predicted by transient absorption experiments. The smaller CdSe quantum dot has still faster cooling, as expected from quantum size effects. The quantum dots of perovskites show extremely fast hot exciton cooling, decaying faster than detection limits of <1 ps, even faster than the CdSe system, suggesting the efficiency of Auger processes in these metal halide perovskite nanocrystals and especially in their quantum dot form. These results across a range of sizes of nanocrystals reveal extremely fast hot exciton cooling at high exciton density, independent of composition, but dependent upon size. Hence these metal halide perovskite nanocrystals seem to cool heavily following quantum dot physics.
Source: openalex_inverted_index · 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

Department of Chemistry, McGill University, Montreal, H3A 0B8, Canada

Institute of Inorganic Chemistry, Department of Chemistry and Applied Biosciences, ETH Zurich, 8093 Zurich, Switzerland

Empa−Swiss Federal Laboratories for Materials Science and Technology, 8600 Dubendorf, Switzerland

Funding

Sony · Canada Foundation for Innovation · Fonds Qu?b?cois de la Recherche sur la Nature et les Technologies · Natural Sciences and Engineering Research Council of Canada · H2020 European Research Council

References (86)

Show source-provided references
1. 10.1021/acs.chemrev.8b0053910.1021/acs.chemrev.8b00539 ↗
2. 10.1038/s41563-018-0018-410.1038/s41563-018-0018-4 ↗
3. 10.1126/science.aam709310.1126/science.aam7093 ↗
4. 10.1021/nl504877910.1021/nl5048779 ↗
5. 10.1021/acsphotonics.2c0139410.1021/acsphotonics.2c01394 ↗
6. 10.1021/acs.nanolett.0c0145210.1021/acs.nanolett.0c01452 ↗
7. 10.1038/ncomms1412010.1038/ncomms14120 ↗
8. 10.1038/nphoton.2015.21310.1038/nphoton.2015.213 ↗
9. 10.1002/adma.20180305410.1002/adma.201803054 ↗
10. 10.1021/acs.jpcc.8b0047610.1021/acs.jpcc.8b00476 ↗
11. 10.1002/adma.20170731210.1002/adma.201707312 ↗
12. 10.1126/science.aaf957010.1126/science.aaf9570 ↗
13. 10.1021/acsenergylett.1c0258110.1021/acsenergylett.1c02581 ↗
14. 10.1038/s41467-020-16463-710.1038/s41467-020-16463-7 ↗
15. 10.1126/sciadv.aax362010.1126/sciadv.aax3620 ↗
16. 10.1002/adma.20180248610.1002/adma.201802486 ↗
17. 10.1038/ncomms1435010.1038/ncomms14350 ↗
18. 10.1038/s41467-017-01360-310.1038/s41467-017-01360-3 ↗
19. 10.1021/acsnano.2c1222010.1021/acsnano.2c12220 ↗
20. 10.1063/5.014211310.1063/5.0142113 ↗
21. 10.1021/acsnano.0c0890310.1021/acsnano.0c08903 ↗
22. 10.1021/acsenergylett.7b0054710.1021/acsenergylett.7b00547 ↗
23. 10.1021/acsnano.5b0732810.1021/acsnano.5b07328 ↗
24. 10.1038/ncomms905610.1038/ncomms9056 ↗
25. 10.1126/science.aau739210.1126/science.aau7392 ↗
26. 10.1038/s41586-018-0683-010.1038/s41586-018-0683-0 ↗
27. 10.1021/jp994413210.1021/jp9944132 ↗
28. 10.1103/PhysRevB.60.1374010.1103/PhysRevB.60.13740 ↗
29. 10.1103/PhysRevLett.80.402810.1103/PhysRevLett.80.4028 ↗
30. 10.1146/annurev.physchem.58.032806.10453710.1146/annurev.physchem.58.032806.104537 ↗
31. 10.1103/PhysRevLett.95.19640110.1103/PhysRevLett.95.196401 ↗
32. 10.1103/PhysRevB.75.24531110.1103/PhysRevB.75.245311 ↗
33. 10.1103/PhysRevLett.98.17740310.1103/PhysRevLett.98.177403 ↗
34. 10.1021/jp205867310.1021/jp2058673 ↗
35. 10.1021/ar100042810.1021/ar1000428 ↗
36. 10.1021/nl504877910.1021/nl5048779 ↗
37. 10.1038/s41586-018-0683-010.1038/s41586-018-0683-0 ↗
38. 10.1038/nature2514710.1038/nature25147 ↗
39. 10.1021/acs.nanolett.8b0302710.1021/acs.nanolett.8b03027 ↗
40. 10.1038/s41563-019-0364-x10.1038/s41563-019-0364-x ↗
41. 10.1038/s41467-018-05876-010.1038/s41467-018-05876-0 ↗
42. 10.1021/acs.nanolett.7b0006410.1021/acs.nanolett.7b00064 ↗
43. 10.1126/science.abq361610.1126/science.abq3616 ↗
44. 10.1063/5.002797210.1063/5.0027972 ↗
45. 10.1021/acs.nanolett.0c0271410.1021/acs.nanolett.0c02714 ↗
46. 10.1039/D0NR02711A10.1039/D0NR02711A ↗
47. 10.1021/acs.nanolett.8b0086110.1021/acs.nanolett.8b00861 ↗
48. 10.1063/1.514218010.1063/1.5142180 ↗
49. 10.1021/acs.nanolett.0c0510910.1021/acs.nanolett.0c05109 ↗
50. 10.1021/acs.nanolett.8b0208010.1021/acs.nanolett.8b02080 ↗
51. 10.1103/PhysRevLett.94.08740310.1103/PhysRevLett.94.087403 ↗
52. 10.1103/PhysRevB.75.24531110.1103/PhysRevB.75.245311 ↗
53. 10.1021/acs.jpclett.1c0075410.1021/acs.jpclett.1c00754 ↗
54. 10.1021/acs.jpcc.7b0843910.1021/acs.jpcc.7b08439 ↗
55. 10.1021/acs.jpcc.2c0650610.1021/acs.jpcc.2c06506 ↗
56. 10.1021/acs.jpcc.1c0950110.1021/acs.jpcc.1c09501 ↗
57. 10.1103/PhysRevResearch.3.02314710.1103/PhysRevResearch.3.023147 ↗
58. 10.1021/acs.jpcc.0c0546210.1021/acs.jpcc.0c05462 ↗
59. 10.1063/1.47387510.1063/1.473875 ↗
60. 10.1103/PhysRevB.54.484310.1103/PhysRevB.54.4843 ↗
61. 10.1021/acs.jpclett.0c0140710.1021/acs.jpclett.0c01407 ↗
62. 10.1021/jacs.7b0568310.1021/jacs.7b05683 ↗
63. 10.1021/acs.jpcc.8b1121810.1021/acs.jpcc.8b11218 ↗
64. 10.1021/jp502102a10.1021/jp502102a ↗
65. 10.1039/D2NR05698D10.1039/D2NR05698D ↗
66. 10.1103/PhysRevB.77.19532410.1103/PhysRevB.77.195324 ↗
67. 10.1103/PhysRevB.71.20531710.1103/PhysRevB.71.205317 ↗
68. 10.1103/PhysRevB.70.08531610.1103/PhysRevB.70.085316 ↗
69. 10.1103/PhysRevB.80.08131010.1103/PhysRevB.80.081310 ↗
70. 10.1021/jz300239j10.1021/jz300239j ↗
71. 10.1021/acs.nanolett.8b0047010.1021/acs.nanolett.8b00470 ↗
72. 10.1063/1.315726910.1063/1.3157269 ↗
73. 10.1021/acsnano.8b0664910.1021/acsnano.8b06649 ↗
74. 10.1063/1.356106310.1063/1.3561063 ↗
75. 10.1021/acs.jpclett.3c0162710.1021/acs.jpclett.3c01627 ↗
76. 10.1021/jp061595910.1021/jp0615959 ↗
77. 10.1126/science.287.5455.101110.1126/science.287.5455.1011 ↗
78. 10.1073/pnas.202226811810.1073/pnas.2022268118 ↗
79. 10.1038/s42005-023-01169-110.1038/s42005-023-01169-1 ↗
80. 10.1016/0038-1098(94)00760-810.1016/0038-1098(94)00760-8 ↗
81. 10.1103/PhysRevB.74.23532810.1103/PhysRevB.74.235328 ↗
82. 10.1021/nn507486810.1021/nn5074868 ↗
83. 10.1021/acs.jpcc.2c0659110.1021/acs.jpcc.2c06591 ↗
84. 10.1038/s41467-019-12830-110.1038/s41467-019-12830-1 ↗
85. 10.1021/acs.nanolett.3c0397510.1021/acs.nanolett.3c03975 ↗
86. 10.1063/5.017336910.1063/5.0173369 ↗