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Properties of the β-delayed proton decay of ^146Ho

The proton-rich isotope 146Ho was produced via the fusion-evaporation reaction ^92Mo (^58Ni, 3p1n). The β-delayed proton decay of 146Ho was studied by proton-γ coincidence measurements using a He-jet tape transport system. The γ-transitions in ^145Tb following the proton emissions were observed, and...

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Bibliographic Details
Published in:Chinese physics C 2010-08, Vol.34 (8), p.1082-1084
Main Author: 马飞 周小红 郑勇 徐树威 谢元祥 陈亮 雷祥国 郭应祥 张玉虎 李占奎 郭松 丁兵 周厚兵 李广顺 王海霞
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Language:English
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Summary:The proton-rich isotope 146Ho was produced via the fusion-evaporation reaction ^92Mo (^58Ni, 3p1n). The β-delayed proton decay of 146Ho was studied by proton-γ coincidence measurements using a He-jet tape transport system. The γ-transitions in ^145Tb following the proton emissions were observed, and the β-delayed proton branching ratios to the final states in the grand-daughter nucleus ^145Tb were determined. According to the relative branching ratios, the ground-state spin of 146Ho has been proposed and the possible configuration discussed.
ISSN:1674-1137
0254-3052
2058-6132
DOI:10.1088/1674-1137/34/8/008