Abstract
We have studied detailed nucleosynthesis in the shocked surface layers of an oxygen-neon-magnesium corecollapse supernova with an eye to determining whether the conditions are suitable for r-process nucleosynthesis. We find no such conditions in an unmodified model, but do find overproduction of N = 50 nuclei (previously seen in early neutron-rich neutrino winds) in amounts that, if ejected, would pose serious problems for Galactic chemical evolution.
| Original language | English |
|---|---|
| Journal | The Astrophysical Journal |
| Volume | 676 |
| Issue number | 2 PART 2 |
| DOIs | |
| Publication status | Published - 2008 |
| Externally published | Yes |
Keywords
- Abundances
- Nuclear reactions
- Nucleosynthesis
- Supernovae: General
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