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Influence of axial energy spread on the negative-mass instability in a relativistic nonneutral E-layer

Technical Report ·
OSTI ID:5670610
This paper investigates the influence of an axial energy spread on the negative-mass instability in a relativistic nonneutral E-layer aligned parallel to a uniform axial magnetic field (B sub 0)(e sub z). The stability analysis is carried out within the framework of the linearized Vlasov-Maxwell equations. It is assumed that the E-layer is thin with radial thickness much smaller than the mean radius and that nu gamma sub 0 << 1, where nu is Budker's parameter and gamma sub 0 mc-squared is the mean electron energy. Stability properties are investigated for the choice of electron distribution function in which all electrons have the same value of canonical angular momentum and a step-function distribution in axial momentum p sub z. The negative-mass growth rate is calculated including the important stabilizing influence of axial energy spread, and it is shown that modest energy spread is sufficient to stabilize perturbations with axial wavenumber.
Research Organization:
Maryland Univ., College Park (USA). Dept. of Physics and Astronomy
OSTI ID:
5670610
Report Number(s):
AD-A-070484
Country of Publication:
United States
Language:
English