In a rarefied gas is a very large number and
is very
small; let us say, to fix ideas, that we have a box whose volume is
at room temperature and atmospheric pressure. Then
and
and (from
Eq. (2.70)) for small
we have
; at the same time the difference between
and
can be
neglected and the volume occupied by the particles (
) is very small so that the collision between two
selected particles is a rather rare event. In this spirit, the
Boltzmann-Grad limit has been suggested as a procedure to obtain a
closure for Eq. (2.70):
and
in
such a way that
remains finite. We stress the fact that
(as seen in section 2.1.2) the total number of collisions
in the unit of time is given by the total scattering cross section
multiplied by
, which for a system of hard spheres gives
. The Boltzmann-Grad limit, therefore, states that the single
particle collision probability must vanish, but the total number of
collisions remains of order
.
Within this limit, the BBGKY hierarchy reads:
where the arguments of and of
are the same as
above, except that the position of the
particle
(
and
) is equal to
(as
). Eq. (2.72) gives a complete
description of the time evolution of a Boltzmann gas (i.e. the ideal
gas obtained in the Boltzmann-Grad limit), usually called the
Boltzmann hierarchy.
Finally the Boltzmann equation is obtained if the molecular chaos assumption is taken into account:
for particles that are about to collide (that is when
and
). This assumption naturally
stems from the Boltzmann-Grad limit, as it is reasonable that, in the
limit of vanishing single-particle collision rate, two colliding
particles are uncorrelated. The lack of correlation of colliding
particles is the essence of the molecular chaos assumption. We
underline that nothing is said about correlation of particles that
have just collided.
With the assumption (2.73) we can rewrite the first
equation of the hierarchy (2.72), omitting the
subscript for simplicity:
with
,
,
.
This represents the Boltzmann equation for hard spheres. We also
observe that the integral in Eq. (2.74) is
extended to the hemisphere
but could be equivalently extended to
the entire sphere
provided a factor
is inserted in front
of the integral itself, as changing
does not change the integrand.
From a rigorous point of view [58], the molecular chaos
has to be assumed and cannot be proved. However it has been
demonstrated that if the Boltzmann hierarchy has a unique solution for
data that satisfy for a generalized form of chaos assumption:
than Eq. (2.75) holds at any time and therefore the
Boltzmann equation is fully justified. Otherwise it has also been
proved that if Eq. (2.75) is satisfied at and
the Boltzmann equation (2.74) admits a solution
for the given initial data, then the Boltzmann hierarchy
(2.72) has at least a solution which satisfy
(2.75) at any time
.