Nuclear weak-interaction processes in stars
| dc.creator | Langanke, K. | |
| dc.creator | Martinez-Pinedo, G. | |
| dc.date | 2002-03-26 | |
| dc.date | 2002-09-16 | |
| dc.date.accessioned | 2026-07-07T11:32:37Z | |
| dc.date.available | 2026-07-07T11:32:37Z | |
| dc.description | Recent experimental data and progress in nuclear structure modeling have lead to improved descriptions of astrophysically important weak-interaction processes. The review discusses these advances and their applications to hydrostatic solar and stellar burning, to the slow and rapid neutron-capture processes, to neutrino nucleosynthesis, and to explosive hydrogen burning. Special emphasis is given to the weak-interaction processes associated with core-collapse supernovae. Despite some significant progress, important improvements are still warranted. Such improvements are expected to come from future radioactive ion-beam facilities. | |
| dc.description | 45 pages, 33 figures, REVTeX 4, submitted to Rev. Mod. Phys., modified following referee's comments | |
| dc.identifier | https://arxiv.org/abs/nucl-th/0203071 | |
| dc.identifier | http://arxiv.org/abs/nucl-th/0203071 | |
| dc.identifier | Rev.Mod.Phys.75:819-862,2003 | |
| dc.identifier | doi:10.1103/RevModPhys.75.819 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/197660 | |
| dc.subject | Nuclear Theory | |
| dc.subject | Astrophysics | |
| dc.title | Nuclear weak-interaction processes in stars | |
| dc.type | text |