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水的分子模型中表面冻结的计算研究。

Computational investigation of surface freezing in a molecular model of water.

作者信息

Haji-Akbari Amir, Debenedetti Pablo G

机构信息

Department of Chemical and Biological Engineering, Princeton University, Princeton, NJ 08544.

Department of Chemical and Biological Engineering, Princeton University, Princeton, NJ 08544

出版信息

Proc Natl Acad Sci U S A. 2017 Mar 28;114(13):3316-3321. doi: 10.1073/pnas.1620999114. Epub 2017 Mar 14.

Abstract

Water freezes in a wide variety of low-temperature environments, from meteors and atmospheric clouds to soil and biological cells. In nature, ice usually nucleates at or near interfaces, because homogenous nucleation in the bulk can only be observed at deep supercoolings. Although the effect of proximal surfaces on freezing has been extensively studied, major gaps in understanding remain regarding freezing near vapor-liquid interfaces, with earlier experimental studies being mostly inconclusive. The question of how a vapor-liquid interface affects freezing in its vicinity is therefore still a major open question in ice physics. Here, we address this question computationally by using the forward-flux sampling algorithm to compute the nucleation rate in a freestanding nanofilm of supercooled water. We use the TIP4P/ice force field, one of the best existing molecular models of water, and observe that the nucleation rate in the film increases by seven orders of magnitude with respect to bulk at the same temperature. By analyzing the nucleation pathway, we conclude that freezing in the film initiates not at the surface, but within an interior region where the formation of double-diamond cages (DDCs) is favored in comparison with the bulk. This, in turn, facilitates freezing by favoring the formation of nuclei rich in cubic ice, which, as demonstrated by us earlier, are more likely to grow and overcome the nucleation barrier. The films considered here are ultrathin because their interior regions are not truly bulk-like, due to their subtle structural differences with the bulk.

摘要

水在从流星、大气云层到土壤和生物细胞等各种各样的低温环境中都会结冰。在自然界中,冰通常在界面处或其附近成核,因为只有在深度过冷状态下才能观察到主体中的均匀成核。尽管近端表面对结冰的影响已得到广泛研究,但对于气液界面附近的结冰,在理解上仍存在重大差距,早期的实验研究大多没有定论。因此,气液界面如何影响其附近的结冰问题仍然是冰物理学中的一个主要开放性问题。在这里,我们通过使用前向通量采样算法来计算过冷水独立纳米膜中的成核速率,从而通过计算解决这个问题。我们使用TIP4P/ice力场,这是现有的最好的水的分子模型之一,并观察到在相同温度下,膜中的成核速率相对于主体增加了七个数量级。通过分析成核途径,我们得出结论,膜中的结冰不是从表面开始,而是在内部区域开始,与主体相比,在该区域更有利于双菱形笼(DDC)的形成。反过来,这通过有利于富含立方冰的核的形成来促进结冰,正如我们之前所证明的,这些核更有可能生长并克服成核障碍。这里考虑的膜是超薄的,因为它们的内部区域与主体存在细微的结构差异,并非真正类似主体。

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