Karna Nabin Kumar, Oyarzua Elton, Walther Jens H, Zambrano Harvey A
Universidad de Concepcion, Concepcion, Chile.
Technical University of Denmark, Copenhagen, Denmark and Chair of Computational Science, ETH Zurich, Zurich, Switzerland.
Phys Chem Chem Phys. 2016 Nov 30;18(47):31997-32001. doi: 10.1039/c6cp06155a.
Nanoscale capillarity has been extensively investigated; nevertheless, many fundamental questions remain open. In spontaneous imbibition, the classical Lucas-Washburn equation predicts a singularity as the fluid enters the channel consisting of an anomalous infinite velocity of the capillary meniscus. Bosanquet's equation overcomes this problem by taking into account fluid inertia predicting an initial imbibition regime with constant velocity. Nevertheless, the initial constant velocity as predicted by Bosanquet's equation is much greater than those observed experimentally. In the present study, large scale atomistic simulations are conducted to investigate capillary imbibition of water in slit silica nanochannels with heights between 4 and 18 nm. We find that the meniscus contact angle remains constant during the inertial regime and its value depends on the height of the channel. We also find that the meniscus velocity computed at the channel entrance is related to the particular value of the meniscus contact angle. Moreover, during the subsequent visco-inertial regime, as the influence of viscosity increases, the meniscus contact angle is found to be time dependent for all the channels under study. Furthermore, we propose an expression for the time evolution of the dynamic contact angle in nanochannels which, when incorporated into Bosanquet's equation, satisfactorily explains the initial capillary rise.
纳米尺度的毛细现象已得到广泛研究;然而,许多基本问题仍未解决。在自发吸渗过程中,经典的卢卡斯 - 沃什伯恩方程预测,当流体进入由毛细弯月面异常无限速度组成的通道时会出现奇点。博赞奎特方程通过考虑流体惯性来克服这个问题,预测了一个具有恒定速度的初始吸渗阶段。然而,博赞奎特方程预测的初始恒定速度远大于实验观测值。在本研究中,进行了大规模原子模拟,以研究水在高度为4至18纳米的狭缝二氧化硅纳米通道中的毛细吸渗现象。我们发现,在惯性阶段弯月面接触角保持恒定,其值取决于通道的高度。我们还发现,在通道入口处计算得到的弯月面速度与弯月面接触角的特定值有关。此外,在随后的粘滞 - 惯性阶段,随着粘度影响的增加,发现对于所有研究的通道,弯月面接触角都与时间有关。此外,我们提出了一个纳米通道中动态接触角随时间演化的表达式,将其纳入博赞奎特方程后,能令人满意地解释初始毛细上升现象。