journal article·2019-04-12

Triplet-Sensitization by Lead Halide Perovskite Thin Films for Near-Infrared-to-Visible Upconversion

Lea Nienhaus, Juan-Pablo Correa-Baena, Sarah Wieghold, Markus Einzinger, Ting-An Lin, Katherine E. Shulenberger, Nathan D. Klein, Mengfei Wu, Vladimir Bulović, Tonio Buonassisi, Marc A. Baldo, Moungi G. Bawendi

ACS Energy Letters· Volume 4· Issue 4
Publisher page

Abstract

Lead halide-based perovskite thin films have attracted great attention due to the rapid increase in perovskite solar cell efficiencies. The same optoelectronic properties that make perovskites ideal absorber materials in solar cells are also beneficial in other light-harvesting applications and make them prime candidates as triplet sensitizers in upconversion via triplet–triplet annihilation in rubrene. In this contribution, we take advantage of long carrier lifetimes and carrier diffusion lengths in perovskite thin films, their high absorption cross-sections throughout the visible spectrum, and the strong spin–orbit coupling owing to the abundance of heavy atoms to sensitize the upconverter rubrene. Employing bulk perovskite thin films as the absorber layer and spin-mixer in inorganic/organic heterojunction upconversion devices allows us to forego the passivating ligands required for colloidal sensitizers, which can hinder exciton transport through large scale arrays and reduce the triplet transfer efficiency to the annihilator. Our bilayer device exhibits an upconversion efficiency in excess of 3% under 785 nm illumination at an incident power of ∼88 W/cm2.
Source: openalex_inverted_index · Quality: baseline

Research context

OpenAlex topics: Perovskite Materials and Applications · Luminescence and Fluorescent Materials · Luminescence Properties of Advanced Materials

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

References (72)

Show source-provided references
1. 10.1063/1.173603410.1063/1.1736034 ↗
2. 10.1063/1.150567710.1063/1.1505677 ↗
3. 10.1039/C7NR05416E10.1039/C7NR05416E ↗
4. 10.1002/ange.20160070210.1002/ange.201600702 ↗
5. 10.1039/c0an00144a10.1039/c0an00144a ↗
6. 10.1021/cr400478f10.1021/cr400478f ↗
7. 10.1038/nnano.2014.31710.1038/nnano.2014.317 ↗
8. 10.1021/jz501799m10.1021/jz501799m ↗
9. 10.1039/C4EE02481H10.1039/C4EE02481H ↗
10. 10.1016/j.ccr.2010.01.00310.1016/j.ccr.2010.01.003 ↗
11. 10.1021/acs.nanolett.6b0350310.1021/acs.nanolett.6b03503 ↗
12. 10.1063/1.169904410.1063/1.1699044 ↗
13. 10.1021/jp809971u10.1021/jp809971u ↗
14. 10.1021/jacs.6b0469210.1021/jacs.6b04692 ↗
15. 10.1021/jacs.6b0878310.1021/jacs.6b08783 ↗
16. 10.1021/acs.nanolett.5b0213010.1021/acs.nanolett.5b02130 ↗
17. Nienhaus, L.; Geva, N.; Correa-Baena, J.; Wu, M.; Wieghold, S.; Bulović, V.; Voorhis, T. V.; Baldo, M. A.; Buonassisi, T.; Bawendi, M. G. Solid-State Infrared-to-Visible Upconversion for Sub-Bandgap Sensitization of Photovoltaics. 2018 IEEE 7th World Conference on Photovoltaic Energy Conversion (WCPEC) (A Joint Conference of 45th IEEE PVSC, 28th PVSEC 34th EU PVSEC); IEEE, 2018; pp 3698–3702.10.1109/PVSC.2018.8547686 ↗
18. 10.1039/C7CC03087H10.1039/C7CC03087H ↗
19. 10.1021/jacs.8b1318010.1021/jacs.8b13180 ↗
20. 10.1002/adma.20160427810.1002/adma.201604278 ↗
21. 10.1038/nphoton.2015.22610.1038/nphoton.2015.226 ↗
22. 10.1021/acsnano.7b0202410.1021/acsnano.7b02024 ↗
23. 10.1039/C8DT00419F10.1039/C8DT00419F ↗
24. 10.1021/acs.nanolett.5b0213010.1021/acs.nanolett.5b02130 ↗
25. 10.1063/1.498413610.1063/1.4984136 ↗
26. 10.1002/adfm.20150562310.1002/adfm.201505623 ↗
27. 10.1038/nmat171010.1038/nmat1710 ↗
28. 10.1146/annurev.physchem.54.011002.10374610.1146/annurev.physchem.54.011002.103746 ↗
29. 10.1021/ar800204610.1021/ar8002046 ↗
30. 10.1021/ja809598r10.1021/ja809598r ↗
31. 10.1038/s41560-018-0323-910.1038/s41560-018-0323-9 ↗
32. 10.1002/anie.20130936110.1002/anie.201309361 ↗
33. 10.1021/ic401215x10.1021/ic401215x ↗
34. 10.1002/aenm.20160235810.1002/aenm.201602358 ↗
35. 10.1039/C5EE03435C10.1039/C5EE03435C ↗
36. 10.1021/acs.jpclett.5b0229010.1021/acs.jpclett.5b02290 ↗
37. 10.1021/ja506624n10.1021/ja506624n ↗
38. 10.1126/science.124398210.1126/science.1243982 ↗
39. 10.1126/science.124316710.1126/science.1243167 ↗
40. 10.1002/aenm.20140081210.1002/aenm.201400812 ↗
41. 10.1021/ja412583t10.1021/ja412583t ↗
42. 10.1021/jz401532q10.1021/jz401532q ↗
43. 10.1039/C8TC00455B10.1039/C8TC00455B ↗
44. 10.1021/acsnano.7b0475110.1021/acsnano.7b04751 ↗
45. 10.1063/1.221883310.1063/1.2218833 ↗
46. 10.1002/adom.20160108710.1002/adom.201601087 ↗
47. 10.1039/C5EE02608C10.1039/C5EE02608C ↗
48. 10.1039/C7CC03087H10.1039/C7CC03087H ↗
49. 10.1039/C6CP07592D10.1039/C6CP07592D ↗
50. 10.1039/C8TA09026B10.1039/C8TA09026B ↗
51. 10.1038/srep0778710.1038/srep07787 ↗
52. 10.1126/sciadv.aao310410.1126/sciadv.aao3104 ↗
53. 10.1021/acs.jpcc.7b0377110.1021/acs.jpcc.7b03771 ↗
54. 10.1126/science.aap928210.1126/science.aap9282 ↗
55. 10.1021/acsomega.8b0055510.1021/acsomega.8b00555 ↗
56. Wieghold S. · ArXiv190201371 Cond-Mat Physics physics · 2019
57. 10.1021/acs.jpcc.7b0917810.1021/acs.jpcc.7b09178 ↗
58. 10.1021/jacs.8b0196610.1021/jacs.8b01966 ↗
59. 10.1021/acs.jpclett.7b0054610.1021/acs.jpclett.7b00546 ↗
60. 10.1039/C2TC00329E10.1039/C2TC00329E ↗
61. 10.1039/C6EE03702J10.1039/C6EE03702J ↗
62. 10.1063/1.166977710.1063/1.1669777 ↗
63. 10.1016/0009-2614(69)80122-310.1016/0009-2614(69)80122-3 ↗
64. 10.1103/PhysRevB.1.171610.1103/PhysRevB.1.1716 ↗
65. 10.1002/adma.20130458810.1002/adma.201304588 ↗
66. 10.1063/1.475244510.1063/1.4752445 ↗
67. 10.1038/nphys327710.1038/nphys3277 ↗
68. 10.1039/B913243K10.1039/B913243K ↗
69. 10.1021/jz300012u10.1021/jz300012u ↗
70. 10.1039/C6TC02818G10.1039/C6TC02818G ↗
71. 10.1002/adfm.20150532410.1002/adfm.201505324 ↗
72. 10.1002/adma.1997009030810.1002/adma.19970090308 ↗