Non-Dipolar Components of Neutron Star Magnetic Fields
| dc.contributor.advisor | Wetro, Legesse (PhD) | |
| dc.contributor.author | Kifle, Mekuanint | |
| dc.date.accessioned | 2018-06-28T12:46:10Z | |
| dc.date.accessioned | 2023-11-09T11:24:00Z | |
| dc.date.available | 2018-06-28T12:46:10Z | |
| dc.date.available | 2023-11-09T11:24:00Z | |
| dc.date.issued | 2007-07 | |
| dc.description.abstract | Due to the existence of both observational and theoretical evidences for the presence of non-dipolar NS magnetic fields, it has become more and more clear that neutron stars posses magnetic field structures, which are much more complicated than the simple assumption of a dipolar neutron star (NS) magnetic field. This thesis intends to show the presence of non-dipolar component of the NS magnetic fields as derived from a recent model by kebede[5]. We will derive both the dipolar and non dipolar components of the field separately. We approach the problem by applying Post-Newtonian approximation, to find the angle dependent charge distribution on the surface of the neutron star, which results in the non dipolar components of the NS magnetic field | en_US |
| dc.identifier.uri | http://10.90.10.223:4000/handle/123456789/4697 | |
| dc.language.iso | en | en_US |
| dc.publisher | Addis Ababa University | en_US |
| dc.subject | Neutron Star Magnetic Fields | en_US |
| dc.title | Non-Dipolar Components of Neutron Star Magnetic Fields | en_US |
| dc.type | Thesis | en_US |