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The influence of energy and axial momentum spreads on the cyclotron maser instability in an intense hollow electron beam propagating parallel to a uniform axial magnetic field B0êz is investigated. The stability analysis is carried out within the framework of the linearized Vlasov–Maxwell equations. It is assumed that ν/γ̂≪1, where ν is Budker’s parameter and γ̂mc2 is the characteristic electron energy. Stability properties are investigated for the choice of electron distribution function in which all electrons have a step-function distribution in energy (H=γmc2) and a step-function distribution in axial momentum (pz). The instability growth rate is calculated including the important stabilizing influence of energy spread (ε=Δγ) and axial momentum spread (Δ=Δpz). It is shown that a modest energy spread (ε≈ a few percent) is sufficient to stabilize perturbations with high magnetic harmonic number (s⩾2). Moreover, a relatively small axial momentum spread (Δ/mc≈0.1) can easily stabilize perturbations with axial wavenumber satisfying ‖kc/ωc‖≳0.2, for typical beam parameters of experimental interest.
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Uhm et al. (1979) studied this question.
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