Abstract
To observe the γ rays emitted from the low-lying isomeric state of 229Th (229mTh), we aim to dope fluoride crystals with its precursor 229Pa. In this study, we produced 229Pa by a 30 MeV proton bombardment on 232Th and developed a chemical separation method. The chemical yield of Pa was 93(4)%, and the physical production yield of 229Pa for the proton energy range of 29.0–30.1 MeV was measured to be 9.4(8) MBq/µAh, which was more than 10 times higher than those of 232,230,228,233Pa. These high chemical and production yields will allow us to prepare fluoride crystals having a sufficient amount of 229Pa for the observation of the γ rays of 229mTh.
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Acknowledgements
This experiment was performed at RI Beam Factory operated by RIKEN Nishina Center and CNS, University of Tokyo. This work was supported by JSPS KAKENHI Grant Number 19K23445.
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Shigekawa, Y., Yin, X., Nambu, A. et al. Production and chemical separation of 229Pa toward observation of γ rays of 229mTh. J Radioanal Nucl Chem 333, 1479–1486 (2024). https://doi.org/10.1007/s10967-023-09069-y
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DOI: https://doi.org/10.1007/s10967-023-09069-y