Dynamics of a self-gravitating magnetized neutron source
| dc.creator | Paret, D. Manreza | |
| dc.date | 2008-10-06 | |
| dc.date | 2008-10-15 | |
| dc.date.accessioned | 2026-07-07T10:09:48Z | |
| dc.date.available | 2026-07-07T10:09:48Z | |
| dc.description | The dynamics of a self-gravitating neutron gas in presence of a magnetic field is being studied taking the equation of state of a magnetized neutron gas obtained in a previous study [2]. We work in a Bianchi I spacetime characterized by a Kasner metric, this metric allow us to take into account the anisotropy that introduces the magnetic field. The set of Einstein-Maxwell field equations for this gas becomes a dynamical system in a 4-dimensional phase space. We get numerical solutions of the system. In particular there is a unique point like solution for different initial conditions. Physically this singular solution may be associated with the collapse of a local volume of neutron material within a neutron star. | |
| dc.description | 30 pages, 7 figures, Bachelor Thesis in Theoretical Physics, written in Spanish | |
| dc.identifier | https://arxiv.org/abs/0810.1071 | |
| dc.identifier | http://arxiv.org/abs/0810.1071 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/171436 | |
| dc.subject | Astrophysics | |
| dc.title | Dynamics of a self-gravitating magnetized neutron source | |
| dc.type | text |