chapter 4 section 4.6



RESULTS

  We performed a Gibbs-Duhem integration in the plane starting with an fcc solid and a fluid at the monodisperse hard sphere freezing point. Both systems consisted of 256 particles and were well equilibrated. Using the ghost-growing method of section 4.4 in combination with eqn. 4.18 we found an initial slope of =1400 (50) (in units such that and are unity). This value was used in the first predictor step to go from =0 to finite , where the slope could be directly measured. We evaluated the coexistence line by gradually increasing from one simulation to the next while integrating eqn. 4.10 to determine the pressure. In figure 4.1 the equilibrium pressure is shown as a function of the polydispersity parameter . The slope starts off at a value of =1400 as we obtained from eqn. 4.18 and increases when is increased. At a value of =0.0056 the slope becomes infinite, so we had to invert the integration, taking P as the independent variable. In this case, we can calculate for increasing values of P by applying the same integration scheme to the reciprocal of eqn. 4.10. Surprisingly, the equilibrium curve continues to bend back, approaching =0 at infinite pressure. In the inset of figure 4.1 we rescale the pressure to , which remains finite and follows a straight line as . The fact that is finite in this limit actually allows us to perform simulations at infinite pressure as will be discussed in the next section.
The divergence of the pressure is somewhat misleading. The pressure indeed goes to infinity on a scale characterized by , but when reduced instead by the volume or an average diameter it remains bounded. In fact, in this limit loses its relevance as a length scale because all particle diameters are going to values much smaller than . Scaling by an average diameter (or the volume) makes the interpretation of the results more intuitive because in experiments the important microscopic length scale is the characteristic particle diameter. Consequently, in most of what follows we present our results in terms of (where the angle brackets indicate an isobaric semigrand ensemble average). We choose arbitrarily to use of the solid to perform the reduction; we could just as well have used the fluid value. We will continue to refer to the limit of infinite pressure because this represents a limiting behavior of our isobaric semigrand system. It should be understood that in this case the pressure is infinite on the scale but not on, say, the scale.
Although the parameter shows a maximum as a function of P, the real polydispersity---given in terms of the width of the composition distribution ---does not. This polydispersity s is defined as

In figure 4.2 the reduced pressure is plotted against the polydispersity s in both the fluid and the solid. The equilibrium pressure increases monotonically until at infinite pressure a limiting value of s and is reached. From this plot it becomes immediately clear that the polydispersity of the fluid and the solid at equilibrium can be very different. As reviewed in the introduction of this chapter, this fact, although anticipated, was discounted in previous studies.

 

Figure:  Phase diagram in the plane of volume fraction and polydispersity. Coexisting phases are joined by tie lines, which are not straight because the polydispersity is not an additive variable. The circles represent the endpoints of the coexistence region at , i.e., the terminal polydispersity.

 

Figure: Phase diagram in the plane of reduced number density and polydispersity. Coexisting phases are joined by tie lines, which although curved in reality are rendered straight in this figure.

 

Figure:  Composition distributions for fluid-solid equilibrium at different pressures. In the figures, the leftmost solid curve represents the fluid composition, the rightmost one the solid phase composition. a) for =15. The dotted curve is the imposed (Gaussian) activity distribution. b) for =100. The dotted curve is the imposed (Gaussian) activity distribution. c) for =6400. The dotted line denotes the imposed chemical potential difference function, which is becoming straight at high . d) for .In this limit the diameters are pushed to zero. By dividing them by they remain finite. The dotted line denotes the imposed chemical potential difference function.


It is convenient to choose a density variable given in terms of the real volume fraction, because this is the quantity one measures in experiments. We define ; note that =0.7405 for monodisperse close packed spheres. The phase diagram in the plane is shown in figure 4.3. Because the polydispersity variable is not linearly additive, the tie-lines are curved. A system of hard spheres prepared on one of the tie-lines will split into a solid and liquid phase with density and polydispersity given by the intersection of the tie-line with the coexistence lines. The most remarkable feature of the diagram is the fact that the fluid-solid equilibrium suddenly ends. This is generally consistent with the prediction and observation of a terminal polydispersity reported in studies on crystallization of polydisperse hard spheres [8,83,82] and reviewed in section 4.1. In particular, the consensus of a terminal polydispersity in the range of 5%--12% is explained by our results. According to our phase diagram, the fcc solid phase is thermodynamically stable for polydispersities no more than 5.7%, yet crystallization is possible in fluids of polydispersity up to 12% provided one allows for fractionation in the phase separation process. This is consistent with Pusey's experiments [8] in which he observed that dispersions with a polydispersity of 7.5% would freeze, while those with a polydispersity of 12% did not. The DFT studies which reported a terminal polydispersity of 5--7% are also consistent with our results given their use of the constrained eutectic, which precludes fractionation.
In figure 4.4, we plot the number density (in units of the average diameter) as a function of s. This plot illustrates the counterintuitive result that the fluid density may adopt values greater than that in the solid phase. At the point where both densities are equal the term in eqn. 4.10 switches sign and becomes negative, which gives rise to the maximum of seen in figure 4.1. Of course, the fluid is able to take on larger densities than the solid only because it is composed of particles of smaller diameter.
The composition distributions of the fluid and the solid phases are displayed in figure 4.5 for four values of the coexistence pressure. For a monodisperse equilibrium (not shown in the figures) the distributions in both phases would be equal to the imposed activity, which is a delta function at . As the equilibrium pressure (or equivalently the value of ) is increased, the composition distributions depart from the ideal activity. Although still almost Gaussian, they are shifted considerably to lower values of . The average diameter is smaller in the fluid, whereas the solid composition is located at larger diameters and is more narrowly distributed. The difference between the phases becomes more pronounced at higher pressures. At infinite pressure, all diameters go to zero on the scale of . Interesting distributions can be recovered by proper scaling of the diameters by their average, as presented in figure 4.5d. The fluid distribution is much broader than the solid one, in accord with the larger polydispersity s we encountered above. Although the value has decreased to zero in this limit (and of course has the same value in the two phases), the (rescaled) composition distributions are still near-Gaussian with a finite width (on a scale of ). This curious outcome is a result of the limiting process in which while .
As the distributions are shifted to lower diameter at high pressure, the precise shape of the imposed activity distribution becomes less important and , as discussed above, becomes irrelevant. In figure 4.5c the chemical potential difference function, the logarithm of the activity, is nearly a straight line; it becomes exactly a straight line in the infinite pressure limit. This property enables us to perform simulations in the limit of .



chapter 4 section 4.6


Peter Bolhuis
Tue Sep 24 20:44:02 MDT 1996