Abstract
Neutron capture cross sections are the key nuclear physics input to study the slow neutron capture process, which is responsible for forming about half of the elemental abundances above Fe. Stellar neutron capture cross section can be measured by the time-of-flight technique, or by activation. Both techniques will be discussed and recent experiments in the Fe/Ni mass region will be presented.
| Original language | English |
|---|---|
| Article number | 012020 |
| Journal | Journal of Physics: Conference Series |
| Volume | 665 |
| Issue number | 1 |
| DOIs | |
| Publication status | Published - 5 Jan 2016 |
| Externally published | Yes |
| Event | 6th Nuclear Physics in Astrophysics, NPA 2013 - Lisbon, Portugal Duration: 19 May 2013 → 24 May 2013 |
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