The rate of decrease in the number of species- particles located between
and
,
and having velocities in the range
to
, due to scattering of species-
particles by species-
particles is
obtained by multiplying
by the the relative flux,
,
of species-
particles incident on a species-
particle, then multiplying by the number of species-
particles,
, that can do the scattering, and, finally, summing over all possible
species-
initial velocities, and all possible species-
and species-
final velocities.
In other words,
In writing the previous expression, we have assumed that the distribution functions and
are uncorrelated. This assumption is reasonable provided that the mean-free-path is much longer than the effective range of
the inter-particle force. (This follows because, before they encounter one another, two colliding particles originate at different points that are typically separated by
a mean-free-path. However, the typical correlation length is of similar magnitude to the range of the inter-particle force.)
In writing the previous expression, we have also implicitly assumed that the inter-particle force responsible for the collisions is sufficiently short-range that
the particle position vectors do not change appreciably (on a macroscopic lengthscale) during a collision. (Both of the previous
assumptions are valid in a conventional weakly coupled plasma because the range of the inter-particle force is of order the Debye
length, which is assumed to be much smaller than any macroscopic lengthscale. Moreover, the mean-free-path is much
longer than the Debye length—see Section 1.7.)
By analogy with Equation (3.19), the rate of increase in the number of species- particles located between
and
,
and having velocities in the range
to
, due to the recoil of species-
particles that scatter species-
particles is
The net rate of change of the distribution function of species- particles with velocities
(at position
and time
) due to collisions with
species-
particles [i.e., the collision operator—see Equation (3.9)] is given by
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(3.22) |
Expression (3.23) for the Boltzmann collision operator can be further simplified for
elastic collisions because, in this case, the collision cross-section
is a function only of the magnitude of the relative velocity vector,
, and its change in direction as a result of the collision. Furthermore, the integral over the final velocities
and
reduces
to an integral over all solid angles for the change in direction of
. Thus,
we can write