2002
DOI: 10.1017/s0263034602204164
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Nonlinear δf simulation studies of intense charged particle beams with large temperature anisotropy

Abstract: This article extends previous numerical studies of the stability properties of intense nonneutral charged particle beams with large temperature anisotropy~T 4b Ͼ Ͼ T 5b ! to allow for nonaxisymmetric perturbations with ]0]u 0. The most unstable modes are identified, and their eigenfrequencies, radial mode structure, and nonlinear dynamics are determined.

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Cited by 18 publications
(27 citation statements)
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“…Of particular importance at the high beam currents and charge densities of practical interest are the effects of the intense self-fields produced by the beam space charge and current on determining the detailed equilibrium, stability, and transport properties. While considerable progress has been made in understanding the self-consistent evolution of the beam distribution function, f b x; p; t, and self-generated electric and magnetic fields, E s x; t and B s x; t, in kinetic analyses based on the nonlinear Vlasov-Maxwell equations [1,6 -10], in numerical simulation studies of intense beam propagation [11][12][13][14][15][16][17][18][19][20][21], and in macroscopic warm-fluid models [22 -25], the effects of finite geometry and space-charge effects often make predictions of detailed stability behavior difficult. It is therefore important to develop an improved understanding of fundamental collective stability properties, including the case where a large temperature anisotropy T ?b T kb can drive a Harris-like instability [26,27], familiar in the study of electrically neutral plasmas.…”
Section: Introductionmentioning
confidence: 99%
“…Of particular importance at the high beam currents and charge densities of practical interest are the effects of the intense self-fields produced by the beam space charge and current on determining the detailed equilibrium, stability, and transport properties. While considerable progress has been made in understanding the self-consistent evolution of the beam distribution function, f b x; p; t, and self-generated electric and magnetic fields, E s x; t and B s x; t, in kinetic analyses based on the nonlinear Vlasov-Maxwell equations [1,6 -10], in numerical simulation studies of intense beam propagation [11][12][13][14][15][16][17][18][19][20][21], and in macroscopic warm-fluid models [22 -25], the effects of finite geometry and space-charge effects often make predictions of detailed stability behavior difficult. It is therefore important to develop an improved understanding of fundamental collective stability properties, including the case where a large temperature anisotropy T ?b T kb can drive a Harris-like instability [26,27], familiar in the study of electrically neutral plasmas.…”
Section: Introductionmentioning
confidence: 99%
“…during the acceleration of the charge bunch [10], and can provide the free energy to drive both the electrostatic Harris instability [32][33][34][35][36][37][38][39][40][41][42] and the electromagnetic Weibel instability [39,[43][44][45][46][47][48].…”
Section: B Electrostatic Harris Instability For One-component Beamsmentioning
confidence: 99%
“…In the absence of axial streaming (β j = 0 and β = 0 = β 2 ), the dispersion relation (31) gives directly the fast wave…”
Section: Weibel Instability For Step-function Density Profilesmentioning
confidence: 99%
“…Nonetheless, often with the aid of numerical simulations, there has been considerable recent analytical progress in applying the Vlasov-Maxwell equations to investigate the detailed equilibrium and stability properties of intense charged particle beams. These investigations include a wide variety of collective interaction processes ranging from the electrostatic Harris instability [29][30][31][32][33][34][35] and electromagnetic Weibel instability [36][37][38][39][40][41] driven by large temperature anisotropy with T ⊥b T b in a one-component nonneutral ion beam, to wall-impedance-driven collective instabilities [42][43][44][45], to the dipole-mode two-stream instability for an intense ion beam propagating through a partially neutralizing electron background [45][46][47][48][49][50][51][52][53][54][55][56], to the resistive hose instability [57][58][59][60][61][62][63] and the sausage and hollowing instabilities [64][65][66] for an intense ion beam propagating through a background plasma [67][68][69]…”
Section: Introductionmentioning
confidence: 99%