Long‐time quasilinear evolution of the free‐electron laser instability for a relativistic electron beam propagating through a helical magnetic wiggler
The long‐time quasilinear development of the free‐electron laser instability is investigated for a tenuous electron beam propagating in the z direction through a helical wiggler field B 0=−B̂ cos k 0 z ê x −B̂ sin k 0 z ê y . The analysis neglects longitudinal perturbations (δφ≂0) and is based on...
Gespeichert in:
Veröffentlicht in: | Phys. Fluids; (United States) 1985-08, Vol.28 (8), p.2524-2536 |
---|---|
Hauptverfasser: | , |
Format: | Artikel |
Sprache: | eng |
Schlagworte: | |
Online-Zugang: | Volltext |
Tags: |
Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
|
Zusammenfassung: | The long‐time quasilinear development of the free‐electron laser instability is investigated for a tenuous electron beam propagating in the z direction through a helical wiggler field B
0=−B̂ cos k
0
z
ê
x
−B̂ sin k
0
z
ê
y
. The analysis neglects longitudinal perturbations (δφ≂0) and is based on the nonlinear Vlasov–Maxwell equations for the class of beam distributions of the form f
b
(z,p,t) =n
0δ(P
x
)δ(P
y
)G(z,p
z
,t), assuming ∂/∂x=0=∂/∂y. The long‐time quasilinear evolution of the system is investigated within the context of a simple ‘‘water‐bag’’ model in which the average distribution function G
0( p
z
,t) =(2L)−
1∫
L
−L
d
z G(z,p
z
,t) is assumed to have the rectangular form G
0( p
z
,t) =[2Δ(t)]−
1 for ‖p
z
−p
0(t)‖ ≤Δ(t), and G
0( p
z
,t) =0 for ‖p
z
−p
0(t)‖ >Δ(t). Making use of the quasilinear kinetic equations, a coupled system of nonlinear equations is derived which describes the self‐consistent evolution of the mean electron momentum p
0(t), the momentum spread Δ(t), the amplifying wave spectrum ‖H
k
(t)‖2, and the complex oscillation frequency ω
k
(t) +iγ
k
(t).
These coupled equations are solved numerically for a wide range of system parameters, assuming that the input power spectrum P
k
(t=0) is flat and nonzero for a finite range of wavenumber k that overlaps with the region of k space where the initial growth rate satisfies γ
k
(t=0) >0. To summarize the qualitative features of the quasilinear evolution, as the wave spectrum amplifies it is found that there is a concomitant decrease in the mean electron energy γ0(t)m
c
2=[m
2
c
4+e
2
B̂2/k
2
0 +p
2
0(t)c
2]1
/
2, an increase in the momentum spread Δ(t), and a downshift of the growth rate γ
k
(t) to lower k values. After sufficient time has elapsed, the growth rate γ
k
has downshifted sufficiently far in k space so that the region where γ
k
>0 no longer overlaps the region where the initial power spectrum P
k
(t=0) is nonzero. Therefore, the wave spectrum saturates, and γ0(t) and Δ(t) approach their asymptotic values. |
---|---|
ISSN: | 0031-9171 2163-4998 |
DOI: | 10.1063/1.865415 |