Here we recount the second virial approximation of Koda et al. in
a format that lends itself easily to a generalisation to other
mixtures than the spherocylinder/sphere system. In particular, the following
relations are valid for any kind of hard linear particles with
cylindrical and inversion symmetry.
Let
,
denote the local number
densities of two species of hard particles, with
where
.
The free energy of the mixture at the level of the second virial
approximation is
|
(13) |
with
|
(14) |
and
|
(15) |
where
is the Mayer overlap function for a pair of particles at the given positions.
Since we are dealing with hard particles, except for the
overlap region of the two objects, where .
The local density variations
produce
a free energy difference with respect to the homogeneous density system.
Ideal free energy:
The ideal part of the free energy variation per particle is given by
To study the possible onset of a nematic-smectic transition a periodic
density variation
|
(18) |
is assumed and inserted in . For the term quadratic in
, we have
|
(19) |
with
.
Thus
|
(20) |
where
, and
is the ideal part of the stability matrix.
Excess free energy:
From and we have
|
(21) |
with the overlap integral defined as
|
(22) |
where
denotes the excluded volume centered at .
For linear particles symmetric with respect to
the general overlap integral may be simplified as
|
(23) |
where is now centered at the origin.
Thus the central task in this approach is the calculation of the cosine
transform of the three kinds of excluded volumes,
|
(24) |
For the quadratic term in the expression for the excess free energy density
we have
,
where the matrix elements of
are
|
(25) |
It is convenient here to introduce the volume of the linear particles
and relate it to the volume of the hard spheres, thus:
. Using the total packing fraction
in place of
we have
|
(26) |
This is a general result valid for hard particles having cylindrical and
inversion symmetry (
) mixed with hard spheres.
Specific systems made up of
spherocylinders/spheres, ellipsoids/spheres, and fused spheres/spheres
will be considered below. Also, a mixture of ``spheroellipsoids''
and spheres is studied.
The total stability matrix is just
.
The system will become unstable towards smectic demixing if at the
given densities there exists a wave number for which the determinant
becomes zero. An eventual smectic phase will be stable if
.
F. J. Vesely / University of Vienna