Publication | Closed Access
Interplay of collisions with quasilinear growth rates of relativistic electron-beam-driven instabilities in a superdense plasma
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Citations
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References
2005
Year
EngineeringNuclear PhysicsRelativistic PlasmaPlasma SciencePlasma PhysicsElectromagnetic FilamentationSuperdense PlasmaMagnetohydrodynamicsRelativistic Electron-beam-driven InstabilitiesPhysicsElectromagnetic InstabilitiesApplied Plasma PhysicAtomic PhysicsPlasma InstabilityCosmic RayNatural SciencesApplied PhysicsRelativistic Electron BeamsQuasilinear Growth Rates
We focus attention on the rapidly growing electromagnetic instabilities arising in the interaction of intense and relativistic electron beams (REB) with supercompressed thermonuclear fuel. REB-target system is considered neutralized in charge and current with a distribution function including beam and target temperatures. The electromagnetic filamentation (Weibel) instability is first considered analytically in a linear approximation. Relevant growth rates parameters then highlight density ratios between target and particle beams, as well as transverse temperatures. Significant refinements include mode-mode coupling and collisions with target electrons. The former qualify the so-called quasilinear (weakly turbulent) approach. Usually, it produces significantly lower growth rates than the linear ones. Collisions enhance them slightly for kc/omega(p) < 1, and dampen them strongly for kc/omega(p) < 1. In a low temperature target plasma, intrabeam scattering also contributes to the instability taming, while keeping it close to zero in a warm plasma. Our numerical exploration provides further support to the cone-angle configuration (Osaka experiment) with REB penetrating close to the dense core of superdense deuterium + tritium fuel.
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