Nucleosynthesis in early supernova winds III: No significant contribution from neutron-rich pockets
| dc.creator | Hoffman, R. D. | |
| dc.creator | Pruet, J. | |
| dc.creator | Fisker, J. L. | |
| dc.creator | Janka, H. -T. | |
| dc.creator | Burras, R. | |
| dc.creator | Woosley, S. E. | |
| dc.date | 2007-12-18 | |
| dc.date.accessioned | 2026-07-07T08:49:49Z | |
| dc.date.available | 2026-07-07T08:49:49Z | |
| dc.description | Recent nucleosynthesis calculations of Type II supernovae using advanced neutrino transport determine that the early neutrino winds are proton-rich. However, a fraction of the ejecta emitted at the same time is composed of neutron-rich pockets. In this paper we calculate the nucleosynthesis contribution from the neutron-rich pockets in the hot convective bubbles of a core-collapse supernova and show that they do not contribute significantly to the total nucleosynthesis. | |
| dc.description | 4 pages, 2 figures | |
| dc.identifier | https://arxiv.org/abs/0712.2847 | |
| dc.identifier | http://arxiv.org/abs/0712.2847 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/144440 | |
| dc.subject | Astrophysics | |
| dc.title | Nucleosynthesis in early supernova winds III: No significant contribution from neutron-rich pockets | |
| dc.type | text |