Rotational Instabilities in Post-Collapse Stellar Cores
| dc.creator | Brown, David | |
| dc.date | 2000-12-20 | |
| dc.date.accessioned | 2026-07-07T03:25:31Z | |
| dc.date.available | 2026-07-07T03:25:31Z | |
| dc.description | A core-collapse supernova might produce large amplitude gravitational waves if, through the collapse process, the inner core can aquire enough rotational energy to become dynamically unstable. In this report I present the results of 3-D numerical simulations of core collapse supernovae. These simulations indicate that for some initial conditions the post-collapse inner core is indeed unstable. However, for the cases considered, the instability does not produce a large gravitational-wave signal. | |
| dc.description | 12 pages, 10 figures; prepared for the proceedings of the workshop on Astrophysical Sources of Gravitational Radiation | |
| dc.identifier | https://arxiv.org/abs/gr-qc/0012084 | |
| dc.identifier | http://arxiv.org/abs/gr-qc/0012084 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/33744 | |
| dc.subject | General Relativity and Quantum Cosmology | |
| dc.subject | Astrophysics | |
| dc.title | Rotational Instabilities in Post-Collapse Stellar Cores | |
| dc.type | text |