Triplet Exciton Enhanced Radioluminescence of Ga3+/Tb3+ Metallacrown Scintillators for X‐Ray Detection
Source abstract
Abstract
Abstract The increasing demand for radiation detection in many applications has led to demanding requirements for scintillators. Realizing low‐dose, pollution‐free, and reliable X‐ray detection has become a key technical challenge. Here, a triplet‐enhanced lanthanide radioluminescence (RL) material Ga3+/Tb3+ metallacrowns (Tb‐1) is reported. This Tb‐1 crystal emits bright green luminescence under ultraviolet light or X‐ray excitation, and the emission intensity is 286 and 242 times that of Tb3+ in inorganic salt, respectively. Tb‐1 crystal is further passivated by trioctylphosphine oxide (TOPO), and the enhanced RL intensity is equivalent to that of commercial Tl‐doped cesium iodide scintillator. In addition, RL of Tb‐1–TOPO has an extremely narrow full width at half maximum and an excellent linear response to the X‐ray dose rate. The detection limit is calculated to be 0.146 μGy s−1, which is 38 times lower than typical medical imaging doses. Triplet‐enhanced lanthanide RL provides new ideas for replacing scintillators that require high temperature synthesis processes such as inorganic phosphors and ceramics, and provides a new alternative scintillator material for flexible X‐ray monitoring, bioimaging, radiotherapy, and other applications.
Source: crossref · Quality: baseline
Research context
OpenAlex topics: Atomic and Subatomic Physics Research · Luminescence Properties of Advanced Materials · Radiation Detection and Scintillator Technologies
SciVX discovery tags are terminology-based. OpenAlex topics are source-provided classifications.
Affiliations
Institute of Optoelectronic Materials and Devices China Jiliang University Hangzhou 310018 P. R. China
HwaMei Hospital University of Chinese Academy of Sciences Ningbo 315010 P. R. China
Funding
Natural Science Foundation of Zhejiang Province
References (32)
Show source-provided references
1. 10.1038/nature2403210.1038/nature24032 ↗
2. 10.1016/j.nima.2015.08.04110.1016/j.nima.2015.08.041 ↗
3. 10.1002/adom.20140057110.1002/adom.201400571 ↗
4. 10.1002/adma.20180174310.1002/adma.201801743 ↗
5. 10.1038/s41586-018-0451-110.1038/s41586-018-0451-1 ↗
6. 10.1021/acsnano.8b0948410.1021/acsnano.8b09484 ↗
7. 10.1038/s41467-019-08981-w10.1038/s41467-019-08981-w ↗
8. 10.1016/j.ceramint.2019.10.18310.1016/j.ceramint.2019.10.183 ↗
9. 10.1016/j.mser.2019.10051810.1016/j.mser.2019.100518 ↗
10. 10.1016/j.ceramint.2020.01.07910.1016/j.ceramint.2020.01.079 ↗
11. 10.1039/C2CS35069F10.1039/C2CS35069F ↗
12. 10.1039/c3sc22126a10.1039/c3sc22126a ↗
13. 10.1039/C4CS00188E10.1039/C4CS00188E ↗
14. 10.1039/C9CP03041G10.1039/C9CP03041G ↗
15. 10.1039/D0QI01153C10.1039/D0QI01153C ↗
16. 10.1021/jacs.6b0098410.1021/jacs.6b00984 ↗
17. 10.1038/s41586-020-2932-210.1038/s41586-020-2932-2 ↗
18. 10.1038/s41566-020-00744-010.1038/s41566-020-00744-0 ↗
19. 10.1039/c3cp52279b10.1039/c3cp52279b ↗
20. 10.1063/1.183045210.1063/1.1830452 ↗
21. 10.1038/s41467-018-06745-610.1038/s41467-018-06745-6 ↗
22. 10.1021/ja047649e10.1021/ja047649e ↗
23. 10.1038/srep0001810.1038/srep00018 ↗
24. 10.1038/s41377-020-00353-010.1038/s41377-020-00353-0 ↗
25. 10.1021/cr900362e10.1021/cr900362e ↗
26. 10.1016/j.jlumin.2014.03.05310.1016/j.jlumin.2014.03.053 ↗
27. 10.1016/j.apradiso.2017.02.01410.1016/j.apradiso.2017.02.014 ↗
28. 10.1038/s41467-020-18119-y10.1038/s41467-020-18119-y ↗
29. Dujardin C. · IEEE Trans. Energy Convers. · 2018 · 65 · 1977
30. 10.1002/adma.20190471110.1002/adma.201904711 ↗
31. 10.1016/j.matt.2020.04.01710.1016/j.matt.2020.04.017 ↗
32. 10.1038/s41467-020-16034-w10.1038/s41467-020-16034-w ↗