Department of Chemistry, University of Utah, Salt Lake City, Utah 84112-0850, USA.
J Am Chem Soc. 2012 Apr 18;134(15):6650-9. doi: 10.1021/ja210878c. Epub 2012 Apr 5.
Water nanoparticles play an important role in atmospheric processes, yet their equilibrium and nonequilibrium liquid-ice phase transitions and the structures they form on freezing are not yet fully elucidated. Here we use molecular dynamics simulations with the mW water model to investigate the nonequilibrium freezing and equilibrium melting of water nanoparticles with radii R between 1 and 4.7 nm and the structure of the ice formed by crystallization at temperatures between 150 and 200 K. The ice crystallized in the particles is a hybrid form of ice I with stacked layers of the cubic and hexagonal ice polymorphs in a ratio approximately 2:1. The ratio of cubic ice to hexagonal ice is insensitive to the radius of the water particle and is comparable to that found in simulations of bulk water around the same temperature. Heating frozen particles that contain multiple crystallites leads to Ostwald ripening and annealing of the ice structures, accompanied by an increase in the amount of ice at the expense of the liquid water, before the particles finally melt from the hybrid ice I to liquid, without a transition to hexagonal ice. The melting temperatures T(m) of the nanoparticles are not affected by the ratio of cubic to hexagonal layers in the crystal. T(m) of the ice particles decreases from 255 to 170 K with the particle size and is well described by the Gibbs-Thomson equation, T(m)(R) = T(m)(bulk) - K(GT)/(R - d), with constant K(GT) = 82 ± 5 K·nm and a premelted liquid of width d = 0.26 ± 0.05 nm, about one monolayer. The freezing temperatures also decrease with the particles' radii. These results are important for understanding the composition, freezing, and melting properties of ice and liquid water particles under atmospheric conditions.
水纳米粒子在大气过程中起着重要作用,但它们的平衡和非平衡液-冰相变以及它们在冻结时形成的结构尚未完全阐明。在这里,我们使用带有 mW 水模型的分子动力学模拟来研究半径为 1 至 4.7nm 的水纳米粒子的非平衡冻结和平衡融化,以及在 150 至 200K 之间的温度下结晶形成的冰的结构。在粒子中结晶的冰是冰 I 的混合形式,其中立方和六方冰多晶型体的堆叠层的比例约为 2:1。立方冰与六方冰的比例与相同温度下模拟的块状水相比不依赖于水粒子的半径,且相似。加热包含多个晶核的冷冻粒子会导致奥斯特瓦尔德成熟和冰结构退火,同时随着液态水的消耗,冰的量增加,然后粒子最终从混合冰 I 融化到液体,而不会转变为六方冰。纳米粒子的熔化温度 T(m)不受晶体中立方和六方层比例的影响。冰粒子的 T(m)从 255 降至 170K,随粒子尺寸变化,并且很好地由 Gibbs-Thomson 方程描述,T(m)(R) = T(m)(bulk) - K(GT)/(R - d),其中常数 K(GT) = 82 ± 5 K·nm,预熔化的液体宽度 d = 0.26 ± 0.05nm,约一个单层。冻结温度也随粒子半径的增大而降低。这些结果对于理解大气条件下冰和液态水粒子的组成、冻结和融化特性很重要。