Neutrino heating of a shock wave within magnetorotational model
| dc.creator | Gvozdev, A. A. | |
| dc.creator | Ognev, I. S. | |
| dc.date | 2006-11-27 | |
| dc.date.accessioned | 2026-07-07T07:30:57Z | |
| dc.date.available | 2026-07-07T07:30:57Z | |
| dc.description | Based on the magnetorotational model of a supernova explosion with core collapse, we investigate the significant processes of neutrino heating of the supernova shock. These processes should be taken into account in self-consistent modeling, since the neutrino heating mechanism is capable of increasing the explosion efficiency. We show that, even in the presence of a strong magnetic field in the shock formation region, the heating rate is determined with good accuracy by the absorption and emission of neutrinos in direct URCA processes. Moreover, the influence on them of a magnetic field is reduced to insignificant corrections. | |
| dc.description | 5 pages, XIV International Seminar Quarks'2006, St.-Petersburg, Repino, Russia, May 19-25, 2006, to appear in the Proceedings | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0611785 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0611785 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/118583 | |
| dc.subject | Astrophysics | |
| dc.title | Neutrino heating of a shock wave within magnetorotational model | |
| dc.type | text |