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with respect to the directions
v
/
v of the electron velocity
v using spherical harmonics
[4,32,33]
k
v
v
f e
f k (
(
x ,
v , t
) =
x , v , t
)
(9.48)
k = 0
or Legendre polynomials if the direction of the force and the expected inhomogeneity
are parallel to a fixed space direction. Because of the orthogonality of the spherical
harmonics, this approach reduces the Boltzmann equation to a set of equations for the
(tensorial) expansion coefficients f k of rank k where the expansion is frequently trun-
cated after the second term, that is, k
1. Here, f 0 is the isotropic part of the velocity
distribution and the further coefficients represent contributions to the distribution
anisotropy. Different FDM codes have been developed to solve the resulting set of
equationsforstationarydischargeplasmaswithzero,one,ortwospatialdimensionsas
well as for time-dependent plasmas with zero or one spatial dimensions [15,33,34].
As an example for the solution of the spatially 1D electron Boltzmann equation
by means of a multiterm method, the calculated spatial evolution of the isotropic
distribution f 0 (
=
in the cathode-fall region of an abnormal H 2 -Ar-N 2 DC glow
discharge in a deposition reactor is shown where the magnitude of the velocity was
replaced by the kinetic energy U
z , U
)
2 [35]. The solver BOLSIG+ that provides
steady-state solutions of the electron Boltzmann equation is freely available [36]
Figure 9.5.
=
m e v 2
/
10 6
10 6
10 5
10 5
10 4
10 4
10 3
10 3
10 2
10 2
10 1
10 1
10 0
10 0
0
0.6 0.7
50
100
0.5
Potential energy
0.4
150
0.3
200
0.2
250
0.1
0
Cathode
FIGURE 9.5 Spatial behavior of the isotropic distribution f 0 ( z , U )
in the cathode-fall region
of a glow discharge in a gas mixture with 71.5% H 2 , 15.3% Ar, and 13.2% N 2 obtained by a
10-term Boltzmann calculation.
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