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Theory of the resistive hose instability in relativistic electron beams

Journal Article · · Phys. Fluids; (United States)
DOI:https://doi.org/10.1063/1.863170· OSTI ID:5152126
A theory of the resistive hose instability is developed for an infinitely long relativistic electron beam propagating parallel to an applied axial magnetic field. Complete space-charge neutralization by the ambient plasma and paraxial flow (p/sup 2//sub z/>>p/sup 2//sub r/+p/sup 2//sub theta/) are assumed. An integro-differential eigenvalue equation is derived from Vlasov--Maxwell theory for the general case, and this equation is reduced to an ordinary differential equation by using a model in which the class of beam electrons with a given transverse energy displaces as a rigid component. The model introduced spread betatron frequency in a natural way that includes correlations to radial position. Using a variational technique, an approximate dispersion relation is found for arbitrary density profile and is evaluated in closed form for either the Bennett or square profile. Stability properties are illustrated and discussed in detail for a square profile, including the influence of the applied magnetic field (stabilizing), proximity to a conducting guide (stabilizing), and partial current neutralization (destabilizing).
Research Organization:
Naval Surface Weapons Center, White Oak, Silver Spring, Maryland 20910
OSTI ID:
5152126
Journal Information:
Phys. Fluids; (United States), Journal Name: Phys. Fluids; (United States) Vol. 23:8; ISSN PFLDA
Country of Publication:
United States
Language:
English