Abstract
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.
| Original language | English |
|---|---|
| Pages (from-to) | 244-256 |
| Number of pages | 13 |
| Journal | Nuclear Physics A |
| Volume | 592 |
| Issue number | 2 |
| DOIs | |
| State | Published - 18 Sep 1995 |
| Externally published | Yes |
Keywords
- RADIOACTIVITY C(βn) [from Be(Ne, X), E = 110 MeV/nucleon]
- measured delayed-neutron spectra, γn-coin, T, deduced log(ft), B(GT). N deduced levels, β-decay branching ratios. Shell model, psd model space
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