Departamento de Química Física, Facultad de Ciencias Químicas, Universidad Complutense de Madrid , 28040 Madrid, Spain.
J Am Chem Soc. 2013 Oct 9;135(40):15008-17. doi: 10.1021/ja4028814. Epub 2013 Sep 25.
Among all of the freezing transitions, that of water into ice is probably the most relevant to biology, physics, geology, or atmospheric science. In this work, we investigate homogeneous ice nucleation by means of computer simulations. We evaluate the size of the critical cluster and the nucleation rate for temperatures ranging between 15 and 35 K below melting. We use the TIP4P/2005 and the TIP4P/ice water models. Both give similar results when compared at the same temperature difference with the model's melting temperature. The size of the critical cluster varies from ∼8000 molecules (radius = 4 nm) at 15 K below melting to ∼600 molecules (radius = 1.7 nm) at 35 K below melting. We use Classical Nucleation Theory (CNT) to estimate the ice-water interfacial free energy and the nucleation free-energy barrier. We obtain an interfacial free energy of 29(3) mN/m from an extrapolation of our results to the melting temperature. This value is in good agreement both with experimental measurements and with previous estimates from computer simulations of TIP4P-like models. Moreover, we obtain estimates of the nucleation rate from simulations of the critical cluster at the barrier top. The values we get for both models agree within statistical error with experimental measurements. At temperatures higher than 20 K below melting, we get nucleation rates slower than the appearance of a critical cluster in all water of the hydrosphere during the age of the universe. Therefore, our simulations predict that water freezing above this temperature must necessarily be heterogeneous.
在所有的冷冻转变中,水变成冰可能与生物学、物理学、地质学或大气科学最为相关。在这项工作中,我们通过计算机模拟研究了均相冰成核。我们评估了临界团簇的大小和在熔点以下 15 到 35 K 温度范围内的成核速率。我们使用了 TIP4P/2005 和 TIP4P/ice water 模型。当与模型的熔点温度进行相同温度差的比较时,这两个模型给出了相似的结果。临界团簇的大小从熔点以下 15 K 时的约 8000 个分子(半径=4nm)变化到熔点以下 35 K 时的约 600 个分子(半径=1.7nm)。我们使用经典成核理论(CNT)来估计冰-水界面自由能和成核自由能垒。我们从对熔融温度的结果外推得到 29(3) mN/m 的界面自由能。这个值与实验测量和之前对 TIP4P 类模型的计算机模拟的估计值非常吻合。此外,我们还从在势垒顶部的临界团簇的模拟中得到了成核速率的估计值。这两个模型的值在统计误差范围内与实验测量值一致。在熔点以下 20 K 以上的温度下,我们得到的成核速率比宇宙年龄期间水圈中所有水的临界团簇的出现都要慢。因此,我们的模拟预测,在这个温度以上的水冻结必然是异质的。