The putative basis for BGK (Bernstein- Greene-Kruskal mode) waves in the wave frame is the 1D Vlasov equation, e.g.
v ¶ f s / ¶ x - q s /m s [¶ je/ ¶ x · ¶ f s/ ¶ v] = 0
Where f s is any function of the constant of the motion for particles species s. And q s , m s refer respectively to the charges and masses for plasma species s.
We expect the solution to be a function of velocity and potential, i.e. f s (v, j)
With general solution:
f s = f s (v 2 + 2q s j /m s - v s2 )
With no magnetic field present, the only Maxwell equation we need is Poisson's e.g.
¶ 2j/ ¶ x2 = - 4 p e (n e – n i) = - 4 p r
For the Poisson equation one obtains the graph below as one "double layer" solution to the potential equation:
Solution to the potential equation for cold streaming plasma: electric potential vs distance (x)
The applicable constant of the motion (total energy) is:
¶ e/ ¶ m s = v 2 + 2q s j /m s - v s2
Where v s is the streaming velocity.
Cases to consider:
1) Cold, electron-ion streaming plasma,
2) Ion-acoustic solitons and shocks,
We examine case (1) first for which:
f s = A n so d (v 2 + 2q s j /m s - vs2 )
Where A is a normalization constant,
n so is n s the particle species number density at locations where the potential:
j = 0.
v s is the streaming velocity at j = 0.
Where: < vs >] f=0 = v s
To get A we first integrate:
n s = ò -¥ ¥ f s dv
Þ
A n so / 2v
Evaluated at: v = Ö vs 2 - 2q s j /m s
Whence: n s = A n so / 2Ö vs 2 - 2q s j /m s
Expression for number density at any potential j .
Then: n s (j = 0) = n so = A n so / 2 vso
Þ
A = 2 vso
Then the distribution function becomes:
f s = 2 v so n so d (v 2 + 2q s j /m s - vso2 )
And:
n s = n so vso /Ö (vso 2 - 2q s j /m s ) =
n so / Ö (1 - q s j /½m s vso2 )
By the continuity equation:
a) n s vs = const. = n so vso
And the momentum equation:
b) m s ns dvs / dt = q s ns E = -q s ns ¶ j/ ¶ x
Also:
c) ½m s vs2 + q s j = const. = ½m s vso2
Problem:
Combine equations (a), (b) and (c) above to obtain an equation for ns in terms of: vso , n so and q s j .
To be continued...
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