X-Ray Bursts and Proton Captures Close to the Dripline
| dc.creator | Rauscher, T. | |
| dc.creator | Rembges, F. | |
| dc.creator | Schatz, H. | |
| dc.creator | Wiescher, M. | |
| dc.creator | Thielemann, F. -K. | |
| dc.date | 2000-07-28 | |
| dc.date.accessioned | 2026-07-07T01:54:36Z | |
| dc.date.available | 2026-07-07T01:54:36Z | |
| dc.description | The hydrogen-rich accreted envelopes of neutron stars in binary systems are the site for the rapid proton capture nucleosynthethic process (rp-process), which involves nuclei close to the proton dripline. An overview of the relevant reactions and nuclear properties for rp-process studies is given, along with motivations for further experimental nuclear physics studies. | |
| dc.description | 6 pages, 4 figures; Proc. Workshop "The beta Decay, from Weak Interaction to Nuclear Structure", eds. P. Dessagne, A. Michalon, C. Miehe (IRes, Strasbourg 1999), p. 51 | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0007451 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0007451 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/1414 | |
| dc.subject | Astrophysics | |
| dc.title | X-Ray Bursts and Proton Captures Close to the Dripline | |
| dc.type | text |