Supernovae, Landau Levels, and Pulsar Kicks
| dc.creator | Kisslinger, Leonard S. | |
| dc.date | 2006-12-18 | |
| dc.date.accessioned | 2026-07-07T11:22:22Z | |
| dc.date.available | 2026-07-07T11:22:22Z | |
| dc.description | We derive the energy asymmetry given the proto-neutronstar during the time when the neutrino sphere is near the surface of the proto-neutron star, using the modified URCA process. The electrons produced with the anti-neutrinos are in Landau levels due to the strong magnetic field, and this leads to asymmetry in the neutrino momentum, and a pulsar kick. Our main prediction is that the large pulsar kicks start at about 10 s and last for about 10 s, with the corresponding neutrinos correlated in the direction of the magnetic field. | |
| dc.description | 10 pages, seven figures | |
| dc.identifier | https://arxiv.org/abs/hep-ph/0612221 | |
| dc.identifier | http://arxiv.org/abs/hep-ph/0612221 | |
| dc.identifier | Mod.Phys.Lett.A22:2071-2080,2007 | |
| dc.identifier | doi:10.1142/S0217732307025315 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/194546 | |
| dc.subject | High Energy Physics - Phenomenology | |
| dc.title | Supernovae, Landau Levels, and Pulsar Kicks | |
| dc.type | text |