Neutrino-Driven Mass Loading of GRMHD Outflows
| dc.creator | Levinson, Amir | |
| dc.date | 2006-10-15 | |
| dc.date.accessioned | 2026-07-07T10:40:30Z | |
| dc.date.available | 2026-07-07T10:40:30Z | |
| dc.description | A GRMHD model of disk outflows with neutrino-driven mass ejection is presented. The model is used to calculate the structure of the outflow in the sub-slow magnetosonic region and the mass loading of the outflow, under conditions anticipated in the central engines of gamma-ray bursts. It is concluded that magnetic launching of ultra-relativistic polar outflows is in principle possible along low inclination field lines (with respect to the symmetry axis), provided the neutrino luminosity is sufficiently low, $L_ν\simlt10^{52}$ erg s$^{-1}$. | |
| dc.description | 6 pages, 2 figures | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0610447 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0610447 | |
| dc.identifier | AIPConf.Proc.924:26-31,2007 | |
| dc.identifier | doi:10.1063/1.2774834 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/181357 | |
| dc.subject | Astrophysics | |
| dc.title | Neutrino-Driven Mass Loading of GRMHD Outflows | |
| dc.type | text |