Department of Chemical Engineering, University of Massachusetts, Amherst, Massachusetts 01003-9303, USA.
J Chem Phys. 2018 Jan 14;148(2):024502. doi: 10.1063/1.5009099.
The stability of the body-centered cubic (bcc) solid phase of classical hard spheres is of intrinsic interest and is also relevant to the development of perturbation theories for bcc solids of other model systems. Using canonical ensemble Monte Carlo, we simulated systems initialized in a perfect bcc lattice at various densities in the solid region. We observed that the systems rapidly evolved into one of four structures that then persisted for the duration of the simulation. Remarkably, one of these structures was identified as cI16, a cubic crystalline structure with 16 particles in the unit cell, which has recently been observed experimentally in lithium and sodium solids at high pressures. The other three structures do not exhibit crystalline order but are characterized by common patterns in the radial distribution function and bond-orientational order parameter distribution; we refer to them as bcc-di, with i ranging from 1 to 3. We found similar outcomes when employing any of the three single occupancy cell (SOC) restrictions commonly used in the literature. We also ran long constant-pressure simulations with box shape fluctuations initiated from bcc and cI16 initial configurations. At lower pressures, all the systems evolved to defective face-centered cubic (fcc) or hexagonal close-packed (hcp) structures. At higher pressures, most of the systems initiated as bcc evolved to cI16 with some evolving to defective fcc/hcp. High pressure systems initiated from cI16 remained in that structure. We computed the chemical potential of cI16 using the Einstein crystal reference method and found that it is higher than that of fcc by ∼0.5kT-2.5kT over the pressure range studied, with the difference increasing with pressure. We find that the undistorted bcc solid, even with constant-volume and SOC restrictions applied, is so mechanically unstable that it is unsuitable for consideration as a metastable phase or as a reference system for studying bcc phases of other systems. On the other hand, cI16 is a mechanically stable structure that can spontaneously emerge from a bcc starting point but it is thermodynamically metastable relative to fcc or hcp.
体心立方(bcc)固相的稳定性具有内在的研究意义,并且与其他模型系统的 bcc 固体的摄动理论的发展也相关。我们使用正则系综蒙特卡罗模拟了在固态区域的各种密度下初始化为完美 bcc 晶格的系统。我们观察到,系统迅速演变成四种结构中的一种,然后在模拟过程中一直保持这种结构。值得注意的是,其中一种结构被鉴定为 cI16,这是一种具有 16 个粒子的立方晶体结构,最近在高压下的锂和钠固体中实验观察到了这种结构。其他三种结构没有表现出晶体有序性,但具有径向分布函数和键取向有序参数分布中的常见模式;我们将它们称为 bcc-di,其中 i 从 1 到 3。当使用文献中常用的三种单占据单元(SOC)限制中的任何一种时,我们也得到了类似的结果。我们还从 bcc 和 cI16 的初始构型出发,进行了带有盒子形状波动的长恒压模拟。在较低的压力下,所有的系统都演变成有缺陷的面心立方(fcc)或六方密堆积(hcp)结构。在较高的压力下,大多数初始为 bcc 的系统演变成 cI16,有些则演变成有缺陷的 fcc/hcp。从 cI16 开始的高压系统保持在该结构中。我们使用爱因斯坦晶体参考方法计算了 cI16 的化学势,发现它在研究的压力范围内比 fcc 高约 0.5kT-2.5kT,并且随着压力的增加,差异也在增加。我们发现,即使施加了等容和 SOC 限制,未变形的 bcc 固体也由于其机械不稳定性而不适合作为亚稳相或作为研究其他系统的 bcc 相的参考体系。另一方面,cI16 是一种机械稳定的结构,可以自发地从 bcc 起点出现,但相对于 fcc 或 hcp 来说,它是热力学亚稳的。