Spin magnetohydrodynamics

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dc.creatorBrodin, G.
dc.creatorMarklund, M.
dc.date2006-12-27
dc.date2007-07-23
dc.date.accessioned2026-07-07T11:24:09Z
dc.date.available2026-07-07T11:24:09Z
dc.descriptionStarting from the non-relativistic Pauli description of spin-1/2 particles, a set of fluid equations, governing the dynamics of such particles interacting with external fields and other particles, is derived. The equations describe electrons, positrons, holes, and similar conglomerates. In the case of electrons, the magnetohydrodynamic limit of an electron-ion plasma is investigated. The results should be of interest and relevance both to laboratory and astrophysical plasmas.
dc.description11 pages, minor typos corrected, to appear in New Journal of Physics
dc.identifierhttps://arxiv.org/abs/physics/0612243
dc.identifierhttp://arxiv.org/abs/physics/0612243
dc.identifierNewJ.Phys.9:277,2007
dc.identifierdoi:10.1088/1367-2630/9/8/277
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/195132
dc.subjectPlasma Physics
dc.subjectAstrophysics
dc.titleSpin magnetohydrodynamics
dc.typetext

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