Smashnova Model
| dc.creator | Sivaram, C | |
| dc.date | 2007-07-07 | |
| dc.date.accessioned | 2026-07-07T08:14:32Z | |
| dc.date.available | 2026-07-07T08:14:32Z | |
| dc.description | An alternate model for gamma ray bursts is suggested. For a white dwarf (WD) and neutron star (NS) very close binary system, the WD (close to Mch) can detonate due to tidal heating, leading to a SN. Material falling on to the NS at relativistic velocities can cause its collapse to a magnetar or quark star or black hole leading to a GRB. As the material smashes on to the NS, it is dubbed the Smashnova model. Here the SN is followed by a GRB. NS impacting a RG (or RSG) (like in Thorne-Zytkow objects) can also cause a SN outburst followed by a GRB. Other variations are explored. | |
| dc.identifier | https://arxiv.org/abs/0707.1091 | |
| dc.identifier | http://arxiv.org/abs/0707.1091 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/133155 | |
| dc.subject | Astrophysics | |
| dc.title | Smashnova Model | |
| dc.type | text |