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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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Published in: | Chinese physics C 2010-08, Vol.34 (8), p.1082-1084 |
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Main Author: | |
Format: | Article |
Language: | English |
Subjects: | |
Online Access: | Get full text |
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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. |
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ISSN: | 1674-1137 0254-3052 2058-6132 |
DOI: | 10.1088/1674-1137/34/8/008 |