Topology of magnetic helicity of torsioned filaments in Hall plasmas
| dc.creator | de Andrade, L. C. Garcia | |
| dc.date | 2007-10-25 | |
| dc.date.accessioned | 2026-07-07T08:38:32Z | |
| dc.date.available | 2026-07-07T08:38:32Z | |
| dc.description | A solution of magnetic Hall equations for plasma filaments in the Coulomb gauge is obtained in the non-holonomic frame. Some physical features of the solution include, the non-conservation of the magnetic helicity and the decay of the magnetic field in the filaments. From the mathematical point of view,the presence of Frenet torsion in the filament is actually shown to be fundamental for the breaking of conservation of magnetic helicity in the case of helicoidal filaments. Since the magnetic helicity is not conserved even in the Coulomb gauge, and the magnetic field decays, one can say that the dynamo action fails. Actually the presence of torsion enhances the breaking of magnetic field helicity conservation. A similar formula of the one obtained here without considering the Hall effect has been obtained by Moffatt and Ricca (PRSA-1992) in the case of holonomic filaments. It is shown that unknotted magnetic filaments may place a lower bound on the magnetic energy. Discussions on the writhe number are also discussed. | |
| dc.description | Deprtamento de Fisica Teorica-IF-UERJ-Rio-Brasil | |
| dc.identifier | https://arxiv.org/abs/0710.4594 | |
| dc.identifier | http://arxiv.org/abs/0710.4594 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/140763 | |
| dc.subject | Astrophysics | |
| dc.title | Topology of magnetic helicity of torsioned filaments in Hall plasmas | |
| dc.type | text |