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Counter-Propagating Beam Instability

As an example of a potentially unstable velocity distribution function, consider

$\displaystyle F_0(u) = n_e\,\frac{v_e}{2\pi}\left[\frac{1}{v_e^{\,2}+(u-V)^{\,2}} + \frac{1}{v_e^{\,2}+(u+V)^{\,2}}\right].$ (8.131)

This function corresponds to two counter-streaming electron beams with so-called Cauchy velocity distributions characterized by the mean velocities $ \pm V$ , and the thermal spreads $ v_e$ . Here,

$\displaystyle n_e = \int_{-\infty}^\infty F_0(u)\,du$ (8.132)

is the electron number density. (It is assumed that there is a stationary background ion fluid of charge density $ e\,n_e$ .) We have seen that a necessary, but not sufficient, criterion for the distribution function (8.131) to be unstable is that it should possess a minimum at finite $ u$ . It is easily demonstrated that this is the case provided $ v_e < \sqrt{3}\,V$ , and, furthermore, that the minimum lies at $ u=0$ . Thus, the system is potentially unstable if $ v_e < \sqrt{3}\,V$ . In order to determine whether the system is actually unstable, we need to evaluate the Penrose condition (8.130) at the minimum. It turns out that the Penrose integral can be evaluated exactly for $ U_0=0$ . In fact,

$\displaystyle \int_{-\infty}^\infty \frac{F_0(u)-F_0(U_0)}{(u-U_0)^{\,2}}\,du = n_e\left[\frac{V^{\,2}- v_e^{\,2}}{(V^{\,2}+ v_e^{\,2})^{\,2}}\right].$ (8.133)

The instability criterion is that this integral be positive, which yields $ v_e < V$ . Assuming that $ k$ is real and positive, it can be shown that, in the small-$ k$ limit, $ k\ll {\mit\Pi}_e/V$ , the growth-rate of the instability is written $ \gamma \equiv -{\rm i}\,\omega \simeq k\,(V-v_e)$ .


next up previous
Next: Current-Driven Ion Acoustic Instability Up: Waves in Warm Plasmas Previous: Velocity-Space Instabilities
Richard Fitzpatrick 2016-01-23