摘要
The β-delayed neutron emission of 19C has been studied with the hope of observing states in 19N close enough to the 18N+n threshold to be of astrophysical significance. Although transitions to three-neutron unbound states in 19N have been observed, no states in the energy region of astrophysical relevance were found. The 19C β-decay branching ratios to the observed states have been measured. All states show log(ft) values typical of allowed transitions. The results are compared with shell-model predictions carried out in the psd model space.
| 源语言 | 英语 |
|---|---|
| 页(从-至) | 244-256 |
| 页数 | 13 |
| 期刊 | Nuclear Physics A |
| 卷 | 592 |
| 期 | 2 |
| DOI | |
| 出版状态 | 已出版 - 18 9月 1995 |
| 已对外发布 | 是 |
指纹
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