Instituto de Química Física Rocasolano, Consejo Superior de Investigaciones Científicas, Calle Serrano 119, 28026 Madrid, Spain.
J Chem Phys. 2010 Jun 21;132(23):234511. doi: 10.1063/1.3454907.
The phase diagram of model anisotropic particles with four attractive patches in a tetrahedral arrangement has been computed at two different values of the range of the potential, with the aim of investigating the conditions under which a diamond crystal can be formed. We find that the diamond phase is never stable for our longer-ranged potential. At low temperatures and pressures, the fluid freezes into a body-centered-cubic solid that can be viewed as two interpenetrating diamond lattices with a weak interaction between the two sublattices. Upon compression, an orientationally ordered face-centered-cubic crystal becomes more stable than the body-centered-cubic crystal, and at higher temperatures, a plastic face-centered-cubic phase is stabilized by the increased entropy due to orientational disorder. A similar phase diagram is found for the shorter-ranged potential, but at low temperatures and pressures, we also find a region over which the diamond phase is thermodynamically favored over the body-centered-cubic phase. The higher vibrational entropy of the diamond structure with respect to the body-centered-cubic solid explains why it is stable even though the enthalpy of the latter phase is lower. Some preliminary studies on the growth of the diamond structure starting from a crystal seed were performed. Even though the diamond phase is never thermodynamically stable for the longer-ranged model, direct coexistence simulations of the interface between the fluid and the body-centered-cubic crystal and between the fluid and the diamond crystal show that at sufficiently low pressures, it is quite probable that in both cases the solid grows into a diamond crystal, albeit involving some defects. These results highlight the importance of kinetic effects in the formation of diamond crystals in systems of patchy particles.
具有四面体排列的四个吸引斑块的各向异性模型粒子的相图已在两种不同的势范围值下进行了计算,目的是研究可以形成金刚石晶体的条件。我们发现,对于我们较长程的势,金刚石相从未稳定。在低温和低压下,流体冻结成体心立方固体,可以看作是两个相互渗透的金刚石晶格,两个子晶格之间存在弱相互作用。在压缩过程中,取向有序的面心立方晶体比体心立方晶体更稳定,在较高的温度下,由于取向无序导致的熵增加稳定了塑性面心立方相。对于较短程的势也发现了类似的相图,但在低温和低压下,我们还发现了一个区域,其中金刚石相在热力学上优于体心立方相。与体心立方固体相比,金刚石结构的较高振动熵解释了为什么即使后者的焓较低,它也稳定。对从晶种开始生长金刚石结构进行了一些初步研究。尽管对于较长程模型,金刚石相在热力学上从未稳定,但对流体和体心立方晶体之间以及流体和金刚石晶体之间界面的直接共存模拟表明,在足够低的压力下,在这两种情况下,固体都很可能生长成金刚石晶体,尽管涉及一些缺陷。这些结果强调了在具有斑块粒子的系统中形成金刚石晶体的动力学效应的重要性。