Radiative Decay of- Hole States
- 1 October 1970
- journal article
- research article
- Published by American Physical Society (APS) in Physical Review C
- Vol. 2 (4) , 1365-1370
- https://doi.org/10.1103/physrevc.2.1365
Abstract
Lifetimes were measured for , , and states formed by promoting a particle from the shell to the shell. In , this state occurs at 990-keV excitation and has a mean life of 0.12 ± 0.04 nsec. By taking account of the branching ratio we find that the partial mean life for the transition is 45 ± 16 nsec. which represents an inhibition of 120 relative to the single-particle estimate. In , the hole state occurs at 2010 keV and has a lifetime of 0.8 ± 0.2 nsec. No other branch is observed, so this is the mean life for the transition. It is inhibited by a factor 62 relative to the single-particle estimate. In the state occurs at 2820 keV and the mean life for this transition is less than 0.08 nsec; the inhibition here is less than 18. All of the above rates are consistent with the theoretical model of Kurath and Lawson. From additional data on , we find that the partial mean life for the 612-keV transition is 1.4 nsec. This is 0.06 times the single-particle value and is not explainable in the scheme of Kurath and Lawson.
Keywords
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