摘要
The rapid neutron nucleosynthesis process involves an enormous amount of very exotic neutron-rich nuclei, which represent a theoretical and experimental challenge. Two of the main decay properties that affect the final abundance distribution the most are half-lives and neutron branching ratios. Using fragmentation of a primary 238U beam at GSI we were able to measure such properties for several neutron-rich nuclei from 208Hg to 218Pb. This contribution provides a short update on the status of the data analysis of this experiment, together with a compilation of the latest results published in this mass region, both experimental and theoretical. The impact of the uncertainties connected with the beta-decay rates and with beta-delayed neutron emission is illustrated on the basis of r-process network calculations. In order to obtain a reasonable reproduction of the third r-process peak, it is expected that both half-lives and neutron branching ratios are substantially smaller, than those based on FRDM+QRPA, commonly used in r-process model calculations. Further measurements around N ∼ 126 are required for a reliable modelling of the underlying nuclear structure, and for performing more realistic r-process abundance calculations.
| 源语言 | 英语 |
|---|---|
| 文章编号 | 012045 |
| 期刊 | Journal of Physics: Conference Series |
| 卷 | 665 |
| 期 | 1 |
| DOI | |
| 出版状态 | 已出版 - 5 1月 2016 |
| 已对外发布 | 是 |
| 活动 | 6th Nuclear Physics in Astrophysics, NPA 2013 - Lisbon, 葡萄牙 期限: 19 5月 2013 → 24 5月 2013 |
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