Origin of Low Carrier Mobilities in Halide Perovskites
Source abstract
Abstract
Halide perovskites constitute a new class of semiconductors that hold promise for low-cost solar cells and optoelectronics. One key property of these materials is the electron mobility, which determines the average electron speed due to a driving electric field. Here we elucidate the atomic-scale mechanisms and theoretical limits of carrier mobilities in halide perovskites by performing a comparative analysis of the archetypal compound CH3NH3PbI3, its inorganic counterpart CsPbI3, and a classic semiconductor for light-emitting diodes, wurtzite GaN, using cutting-edge many-body ab initio calculations. We demonstrate that low-energy longitudinal-optical phonons associated with fluctuations of the Pb–I bonds ultimately limit the mobility to 80 cm2/(V s) at room temperature. By extending our analysis to a broad class of compounds, we identify a universal scaling law for the carrier mobility in halide perovskites, and we establish the design principles to realize high-mobility materials.
Source: openalex_inverted_index · Quality: baseline
Research context
OpenAlex topics: Perovskite Materials and Applications · Chalcogenide Semiconductor Thin Films · Optical properties and cooling technologies in crystalline materials
SciVX discovery tags are terminology-based. OpenAlex topics are source-provided classifications.
Affiliations
Department of Materials, University of Oxford, Parks Road, Oxford OX1 3PH, United Kingdom
Department of Materials Science and Engineering, Cornell University, Ithaca, New York 14853, United States
Funding
Engineering and Physical Sciences Research Council · Leverhulme Trust · H2020 Future and Emerging Technologies
References (70)
Show source-provided references
1. 10.1038/nphoton.2014.13410.1038/nphoton.2014.134 ↗
2. 10.1038/nnano.2015.9010.1038/nnano.2015.90 ↗
3. 10.1021/ja809598r10.1021/ja809598r ↗
4. 10.1126/science.122860410.1126/science.1228604 ↗
5. 10.1038/srep0059110.1038/srep00591 ↗
6. 10.1038/nnano.2014.14910.1038/nnano.2014.149 ↗
7. 10.1038/nmat427110.1038/nmat4271 ↗
8. 10.1038/nphoton.2015.24310.1038/nphoton.2015.243 ↗
9. 10.1038/nphoton.2017.9410.1038/nphoton.2017.94 ↗
10. 10.1038/nenergy.2016.18510.1038/nenergy.2016.185 ↗
11. 10.1038/natrevmats.2016.10010.1038/natrevmats.2016.100 ↗
12. 10.1002/adma.20170283810.1002/adma.201702838 ↗
13. 10.1126/sciadv.160193510.1126/sciadv.1601935 ↗
14. 10.1126/science.aaf460310.1126/science.aaf4603 ↗
15. 10.1038/ncomms667810.1038/ncomms6678 ↗
16. 10.1038/s41467-017-02670-210.1038/s41467-017-02670-2 ↗
17. 10.1021/acsenergylett.7b0027610.1021/acsenergylett.7b00276 ↗
18. 10.1038/ncomms858610.1038/ncomms8586 ↗
19. 10.1038/srep1274610.1038/srep12746 ↗
20. 10.1039/C6CP01402J10.1039/C6CP01402J ↗
21. 10.1038/srep1996810.1038/srep19968 ↗
22. 10.1039/C8TC04750B10.1039/C8TC04750B ↗
23. 10.1103/PhysRevB.97.12120110.1103/PhysRevB.97.121201 ↗
24. 10.1002/adfm.20150234010.1002/adfm.201502340 ↗
25. 10.1021/acs.jpclett.5b0248510.1021/acs.jpclett.5b02485 ↗
26. 10.1126/science.aaa272510.1126/science.aaa2725 ↗
27. 10.1126/science.aaa576010.1126/science.aaa5760 ↗
28. 10.1021/acs.jpcc.8b0034110.1021/acs.jpcc.8b00341 ↗
29. 10.1002/aelm.20150000810.1002/aelm.201500008 ↗
30. 10.1038/ncomms1394110.1038/ncomms13941 ↗
31. 10.1063/1.12101710.1063/1.121017 ↗
32. 10.1016/0038-1101(77)90054-510.1016/0038-1101(77)90054-5 ↗
33. 10.1021/ic401215x10.1021/ic401215x ↗
34. 10.1021/acs.jpclett.6b0254210.1021/acs.jpclett.6b02542 ↗
35. 10.1021/acs.jpca.7b1155810.1021/acs.jpca.7b11558 ↗
36. 10.1039/C4CC09944C10.1039/C4CC09944C ↗
37. 10.1002/adma.20160001110.1002/adma.201600011 ↗
38. 10.1038/ncomms1225310.1038/ncomms12253 ↗
39. 10.1039/C6MH00275G10.1039/C6MH00275G ↗
40. 10.1103/PhysRevB.96.19520210.1103/PhysRevB.96.195202 ↗
41. 10.1103/PhysRevLett.121.08640210.1103/PhysRevLett.121.086402 ↗
42. 10.1103/RevModPhys.89.01500310.1103/RevModPhys.89.015003 ↗
43. 10.1103/PhysRev.116.52610.1103/PhysRev.116.526 ↗
44. 10.1143/PTP.25.51710.1143/PTP.25.517 ↗
45. 10.1126/sciadv.170121710.1126/sciadv.1701217 ↗
46. 10.1039/C7EE01981E10.1039/C7EE01981E ↗
47. 10.1002/adma.20170731210.1002/adma.201707312 ↗
48. 10.1038/nphys335710.1038/nphys3357 ↗
49. 10.1021/acs.jpclett.6b0256010.1021/acs.jpclett.6b02560 ↗
50. 10.1038/ncomms675710.1038/ncomms6757 ↗
51. 10.1021/acsnano.8b0026710.1021/acsnano.8b00267 ↗
52. 10.1021/acs.jpcc.5b0743210.1021/acs.jpcc.5b07432 ↗
53. 10.1021/acs.jpcc.8b0466910.1021/acs.jpcc.8b04669 ↗
54. 10.1038/ncomms1175510.1038/ncomms11755 ↗
55. 10.1063/1.11967310.1063/1.119673 ↗
56. 10.1109/LED.2017.273765810.1109/LED.2017.2737658 ↗
57. 10.1038/nphoton.2016.4110.1038/nphoton.2016.41 ↗
58. 10.1038/nmat492710.1038/nmat4927 ↗
59. 10.1088/1361-648X/aa8f7910.1088/1361-648X/aa8f79 ↗
60. 10.1103/PhysRevB.88.08511710.1103/PhysRevB.88.085117 ↗
61. 10.1016/j.cpc.2018.01.01210.1016/j.cpc.2018.01.012 ↗
62. 10.1039/c3ta10518k10.1039/c3ta10518k ↗
63. 10.1063/1.136815610.1063/1.1368156 ↗
64. 10.1103/PhysRevB.77.03341810.1103/PhysRevB.77.033418 ↗
65. 10.1016/j.cpc.2009.02.00310.1016/j.cpc.2009.02.003 ↗
66. 10.1103/PhysRevLett.62.116910.1103/PhysRevLett.62.1169 ↗
67. 10.1103/PhysRevB.78.08512510.1103/PhysRevB.78.085125 ↗
68. 10.1016/j.cpc.2016.07.02810.1016/j.cpc.2016.07.028 ↗
69. 10.1016/j.cpc.2014.05.00310.1016/j.cpc.2014.05.003 ↗
70. 10.1021/acs.jpclett.5b0072310.1021/acs.jpclett.5b00723 ↗