Superfluid Hydrodynamics of an Electron Gas in a Superstrong Magnetic Field

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dc.creatorKolomeisky, Eugene B.
dc.date2000-08-24
dc.date.accessioned2026-07-07T02:38:33Z
dc.date.available2026-07-07T02:38:33Z
dc.descriptionWe derive the equations of hydrodynamics of a fully polarized electron gas placed in a strong magnetic field. These equations reveal the existence of solitons - immobile or propagating domain wall-like defects whose plane is perpendicular to the field direction. The solitons are used to construct weakly excited states, and novel nonuniform persistent current states of the system.
dc.description4 paqes, 3 figures
dc.identifierhttps://arxiv.org/abs/cond-mat/0008371
dc.identifierhttp://arxiv.org/abs/cond-mat/0008371
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/16712
dc.subjectCondensed Matter
dc.subjectAstrophysics
dc.titleSuperfluid Hydrodynamics of an Electron Gas in a Superstrong Magnetic Field
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