118 10. PLASMA MODELING
where n
0
denotes the plasma density at the sheath edge. Finally, the Poisson equation must be
fulfilled self-consistently
@
2
ˆ
@x
2
D
e
"
0
@
@x
.n
i
n
e
/: (10.18)
With x D 0 at the electrode surface (see Figs. 6.2 and 6.3), a computational grid is extended to a
sufficient depth x
p
in the plasma. e initial conditions are n
e
.x; 0/ D n
i
.x; 0/ D n
0
, where the
presheath is neglected and thereby the factor e
1=2
is omitted. With the voltage V
0
applied
at t D 0, the above system of equations is solved numerically with the boundary conditions
ˆ.0; t / D V
0
and ˆ.x
p
; t / D 0.
Are result of such a calculation is given in Fig. 10.4, which shows the velocity of the sheath
edge, which moves from the electrode into the plasma volume, vs. the position of the sheath
edge. e results relies on experimental information about the plasma density and the electron
temperature. It is in qualitative agreement with the analytical predictions of Section 6.4, with
a high initial sheath edge velocity which tends to zero when approaching the static Langmuir-
Child sheath. e prediction is in good agreement with experimental results obtained from
time-resolved laser-induced fluorescence at varying distance from the electrode.
10.4 PARTICLE-IN-CELL COMPUTER SIMULATION
e most powerful plasma simulations rely on the so-called “particle-in-cell” (PIC) model. e
plasma volume is subdivided by a two-dimensional or three-dimensional grid. All particles in
the plasma are represented by “superparticles” of each species, which represent a large number
of real particles of that species. e superparticles are allowed to move in the entire volume,
whereas the fields which govern their motion are defined on the nodes of the grid. As indicated
in Fig. 10.5, complicated configurations with superimposed electrical and magnetic fields can
be treated in this way.
e procedure of a particle-in-cell simulation is shown schematically in Fig. 10.6. A com-
putational loop is performed for sufficiently small time step t. Starting with the lower-left
edge, the forces on each particles are calculated by interpolating the fields at the grid nodes j
adjacent to the actual position x
i
of the respective particle. Subsequently, the equation of mo-
tion can be solved for each particle. Particles arriving at the walls are treated according to the
boundary conditions (loss or reemission at the walls) with a possible generation of secondary
particles (secondary electron emission, wall sputtering, surface chemistry products, etc.). Ac-
cording to the individual collision cross sections and the corresponding collision probabilities,
a Monte Carlo algorithm decides according if any particle undergoes a collision with any other
species during the time interval. In case of a collision, the velocities and flight directions of the
collision partners are revised. en, the particle densities of different species can be determined
at each grid node from the particle numbers around that grid node and the respective positions.
Finally, the electrostatic potential and the electric field are obtained from the charged parti-