journal article·2025-06-04

High-Performance X-ray Detection Made of Bismuth Perovskite Single Crystal Based on Hydrogen-Bond-Free and Interlayer-Spacing Engineering Strategies

Guangya Zheng, Bin Song, Ling Xu, Song He, Jincong Pang, Hanchen Li, Tong Jin, Yuanpeng Shi, Zhiping Zheng, Guangda Niu, Haodi Wu, Jiang Tang

ACS Applied Materials & Interfaces· Volume 17· Issue 22
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Abstract

Hybrid organic–inorganic halide perovskites (HPs) show great potential for optoelectronic applications. However, their poor stability against moisture and oxygen significantly limits their practical applications. Developing hybrid perovskites with improved stability is essential yet remains a considerable challenge. Lead-free A 3 Bi 2 I 9 perovskites have become attractive semiconductor materials for next-generation X-ray sensing because of their elevated bulk resistivity, efficient X-ray absorption, and low ion migration. Nonetheless, the increased spacing between lamellae along the c -axis hinders carrier mobility in the vertical orientation, thereby presenting difficulty in enhancing the detection sensitivity of these materials. In this work, we present two practical approaches that offer innovative solutions to the aforementioned challenges. The first approach, termed the “hydrogen-bond elimination” strategy, focuses on improving the stability of low-dimensional (LD) HPs by preventing the organic components from establishing strong hydrogen bonds with external water molecules. The “interlayer-spacing engineering” approach focuses on improving carrier transport in the vertical direction. As a proof-of-concept application, a novel large sterically hindered A-site cation, phenyltrimethylammonium (C 9 H 14 N + ), without hydrogen bonding, is introduced to reduce the interlayer spacing through inducing greater structural distortions. The large (C 9 H 14 N) 3 Bi 2 I 9 single crystals (SCs) grown exhibit reduced interlamellar spacing, resulting in a mobility-lifetime (μτ) product of 8.53 × 10 –3 cm 2 V –1 . This value surpasses that of the top-performing MA 3 Bi 2 I 9 SC by a factor of 3, which has a μτ product of 2.87 × 10 –3 cm 2 V –1 . As a result, X-ray detection devices using (C 9 H 14 N) 3 Bi 2 I 9 SCs demonstrate a remarkable sensitivity of 1373.27 μC Gy air –1 cm –2 under a minimal field strength (5.71 V mm –1 ) and an exceptionally low detection limit (LoD) of 4.69 nGy s –1 . These findings pave the way for creating efficient X-ray detection devices using A 3 Bi 2 I 9 -type perovskite or perovskite-like materials, offering an alternative that avoids the use of toxic elements.
Source: openalex_inverted_index · Quality: baseline

Research context

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

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

Affiliations

Wuhan National Laboratory for Optoelectronics & School of Optical and Electronic Information

Huazhong University of Science and Technology

Research Center for Advanced Detection Materials and Medical Imaging Devices, Shenzhen Institute of Advanced Technology

Chinese Academy of Sciences

Optics Valley Laboratory

Ezhou Industrial Technology Research Institute, Wenzhou Institute of Advanced Manufacturing Technology

JFS Laboratory

Funding

China Association for Science and Technology · National Key Research and Development Program of China · National Postdoctoral Program for Innovative Talents · Huazhong University of Science and Technology · Natural Science Foundation of Hubei Province · Major State Basic Research Development Program of China · National Natural Science Foundation of China · Wuhan National Laboratory for Optoelectronics · Innovation Center of Radiation Application · Wenzhou Science and Technology Innovation Foundation

References (69)

Show source-provided references
1. 10.1038/s41467-019-08981-w10.1038/s41467-019-08981-w ↗
2. 10.1038/s41566-021-00909-510.1038/s41566-021-00909-5 ↗
3. 10.1016/j.matt.2020.11.01510.1016/j.matt.2020.11.015 ↗
4. 10.1038/s41566-023-01154-810.1038/s41566-023-01154-8 ↗
5. 10.1038/nature2403210.1038/nature24032 ↗
6. 10.1038/s41928-021-00644-310.1038/s41928-021-00644-3 ↗
7. 10.1002/eom2.1206410.1002/eom2.12064 ↗
8. 10.1016/j.mattod.2021.01.02810.1016/j.mattod.2021.01.028 ↗
9. 10.1038/s41566-022-01024-910.1038/s41566-022-01024-9 ↗
10. 10.1002/adma.20210307810.1002/adma.202103078 ↗
11. 10.1002/anie.20230243510.1002/anie.202302435 ↗
12. 10.1117/12.38448510.1117/12.384485 ↗
13. 10.1039/D2TC04481A10.1039/D2TC04481A ↗
14. 10.1021/acsami.1c2408610.1021/acsami.1c24086 ↗
15. 10.1002/adma.20200154010.1002/adma.202001540 ↗
16. 10.1002/adfm.20180698410.1002/adfm.201806984 ↗
17. 10.1038/s41467-021-21934-610.1038/s41467-021-21934-6 ↗
18. 10.1038/nphoton.2016.4110.1038/nphoton.2016.41 ↗
19. 10.1038/nphoton.2017.4310.1038/nphoton.2017.43 ↗
20. 10.1002/pssr.20180038010.1002/pssr.201800380 ↗
21. 10.1021/acs.nanolett.1c0070010.1021/acs.nanolett.1c00700 ↗
22. 10.1021/cg400645t10.1021/cg400645t ↗
23. 10.1021/acsami.9b1477210.1021/acsami.9b14772 ↗
24. 10.1039/C9TC05490A10.1039/C9TC05490A ↗
25. 10.1038/s41467-021-21805-010.1038/s41467-021-21805-0 ↗
26. 10.1002/adfm.20210914910.1002/adfm.202109149 ↗
27. 10.1021/acsami.9b0284010.1021/acsami.9b02840 ↗
28. 10.1002/adma.20210656210.1002/adma.202106562 ↗
29. 10.1038/s41566-017-0012-410.1038/s41566-017-0012-4 ↗
30. 10.1002/adma.20180445010.1002/adma.201804450 ↗
31. 10.1002/adma.20200601010.1002/adma.202006010 ↗
32. 10.1002/adma.20200379010.1002/adma.202003790 ↗
33. 10.1002/anie.20200416010.1002/anie.202004160 ↗
34. 10.1002/adfm.20210488010.1002/adfm.202104880 ↗
35. 10.1021/jacs.1c0895910.1021/jacs.1c08959 ↗
36. 10.1021/acsenergylett.7b0044210.1021/acsenergylett.7b00442 ↗
37. 10.1039/C8TC06129G10.1039/C8TC06129G ↗
38. 10.1038/s41566-019-0466-710.1038/s41566-019-0466-7 ↗
39. 10.1016/j.jechem.2020.02.04910.1016/j.jechem.2020.02.049 ↗
40. 10.1016/j.matt.2020.04.01710.1016/j.matt.2020.04.017 ↗
41. 10.1002/adom.20200081410.1002/adom.202000814 ↗
42. 10.1002/adfm.20191064810.1002/adfm.201910648 ↗
43. 10.1002/adma.20210301010.1002/adma.202103010 ↗
44. 10.1002/adfm.20190970110.1002/adfm.201909701 ↗
45. 10.1021/acs.jpclett.1c0009010.1021/acs.jpclett.1c00090 ↗
46. 10.1039/D1QI01049B10.1039/D1QI01049B ↗
47. 10.1038/s41467-020-16034-w10.1038/s41467-020-16034-w ↗
48. 10.1021/ja511132a10.1021/ja511132a ↗
49. 10.1021/acsnano.7b0411610.1021/acsnano.7b04116 ↗
50. 10.1039/C9TC01967G10.1039/C9TC01967G ↗
51. 10.1021/acs.cgd.9b0133810.1021/acs.cgd.9b01338 ↗
52. 10.1039/D4TC00594E10.1039/D4TC00594E ↗
53. 10.1103/PhysRevB.54.1116910.1103/PhysRevB.54.11169 ↗
54. 10.1063/1.156406010.1063/1.1564060 ↗
55. 10.1063/1.220459710.1063/1.2204597 ↗
56. 10.1063/1.487866410.1063/1.4878664 ↗
57. 10.1016/0039-6028(94)00731-410.1016/0039-6028(94)00731-4 ↗
58. 10.1021/acsami.9b1574410.1021/acsami.9b15744 ↗
59. 10.1126/science.172.3983.56710.1126/science.172.3983.567 ↗
60. 10.1002/adma.20150197810.1002/adma.201501978 ↗
61. 10.1039/C5CC10455F10.1039/C5CC10455F ↗
62. 10.1002/pssb.1966015022410.1002/pssb.19660150224 ↗
63. 10.1002/chem.20150505510.1002/chem.201505055 ↗
64. 10.1002/adma.20240612810.1002/adma.202406128 ↗
65. 10.1021/acs.nanolett.4c0085110.1021/acs.nanolett.4c00851 ↗
66. Berger M. · 2013
67. 10.1039/D4CP01318B10.1039/D4CP01318B ↗
68. 10.1002/adma.20221197710.1002/adma.202211977 ↗
69. 10.1021/acs.accounts.5b0042010.1021/acs.accounts.5b00420 ↗