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地下储氢背景下二氧化硅表面的润湿性偏好:分子动力学视角

Wetting Preference of Silica Surfaces in the Context of Underground Hydrogen Storage: A Molecular Dynamics Perspective.

作者信息

Ghafari Mohamad Ali, Ghasemi Mehdi, Niasar Vahid, Babaei Masoud

机构信息

Institute of Petroleum Engineering, School of Chemical Engineering, College of Engineering, University of Tehran, P.O. Box 11365-4563, Tehran 61113411, Iran.

Department of Chemical Engineering, The University of Manchester, Manchester M13 9PL, U.K.

出版信息

Langmuir. 2024 Oct 1;40(39):20559-20575. doi: 10.1021/acs.langmuir.4c02311. Epub 2024 Sep 14.

Abstract

The growing interest in large-scale underground hydrogen (H) storage (UHS) emphasizes the need for a comprehensive understanding of the fundamental characteristics of subsurface environments. The wetting preference of subsurface rock is a crucial parameter influencing the H flow behavior during storage and withdrawal processes. In this study, we utilized molecular dynamics simulation to evaluate the wetting preference of the silica surface in subsurface hydrogen systems, with the aim of addressing disparities observed in experimental results. We conducted an initial comprehensive assessment of potential models, comparing the wettability of five common silica surfaces with different surface morphologies and hydroxyl densities in CO-H/water/silica systems against experimental data. After introducing the INTERFACE force field as the most accurate potential model for the silica surface, we evaluated the wetting behavior of the α-quartz (101) surface with a hydroxyl density of 5.9 number/nm under the impact of actual geological storage conditions (333-413 K and 10-30 MPa), the coexistence of cushion gases (i.e., CO, CH, and N) at various mole fractions, and pH levels ranging from 2 to 11 characterized through considering the negative charges of 0 to -0.12 C/m via deprotonation of silanol on the silica surface. Our results indicate that neither pressure nor temperature has a significant impact on the wetness of the silica in the case of pure H (single component UHS operations). However, when CO coexists with H, especially at higher mole fractions, an increase in pressure and a decrease in temperature lead to higher contact angles. Moreover, when the mole fraction of cushion gas ranges from 0 to 1, the contact angle increases 20, 9.5, and 4.5° for CO, CH, and N, respectively, on the neutral silica substrate. Interestingly, at higher pH conditions where the silica surface carries a negative charge, the contact angle considerably reduces where surface charges of -0.03 and -0.06 C/m result in an average reduction of 20 and 80% in the contact angle, respectively. More importantly, at a pH of ∼11 (-0.12 C/m), a 0° contact angle is observed for the silica surface under all temperatures, pressures, types of cushion gases, and varying mole fractions.

摘要

对大规模地下氢存储(UHS)的兴趣与日俱增,这凸显了全面了解地下环境基本特征的必要性。地下岩石的润湿性是影响存储和提取过程中氢流动行为的关键参数。在本研究中,我们利用分子动力学模拟来评估地下氢系统中二氧化硅表面的润湿性,旨在解决实验结果中观察到的差异。我们对潜在模型进行了初步全面评估,将CO-H/水/二氧化硅系统中具有不同表面形态和羟基密度的五个常见二氧化硅表面的润湿性与实验数据进行了比较。在引入INTERFACE力场作为二氧化硅表面最准确的潜在模型后,我们评估了在实际地质存储条件(333 - 413 K和10 - 30 MPa)、各种摩尔分数的缓冲气体(即CO、CH和N)共存以及通过考虑二氧化硅表面硅醇去质子化产生的0至 - 0.12 C/m负电荷表征的pH值范围为2至11的情况下,羟基密度为5.9个/纳米的α - 石英(101)表面的润湿行为。我们的结果表明,在纯氢(单组分UHS操作)情况下,压力和温度对二氧化硅的润湿性均无显著影响。然而,当CO与H共存时,尤其是在较高摩尔分数下,压力升高和温度降低会导致接触角增大。此外,当中性二氧化硅基底上缓冲气体的摩尔分数范围为0至1时,CO、CH和N的接触角分别增加20°、9.5°和4.5°。有趣的是,在二氧化硅表面带负电荷的较高pH条件下,接触角会大幅减小,表面电荷为 - 0.03和 - 0.06 C/m时,接触角分别平均减小20%和80%。更重要的是,在pH约为11( - 0.12 C/m)时,在所有温度、压力、缓冲气体类型和不同摩尔分数下,二氧化硅表面的接触角均为0°。

https://cdn.ncbi.nlm.nih.gov/pmc/blobs/a260/11447897/19b7fefed522/la4c02311_0001.jpg

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