日本地球惑星科学連合2015年大会

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セッション記号 S (固体地球科学) » S-CG 固体地球科学複合領域・一般

[S-CG60] 流体と沈み込み帯のダイナミクス

2015年5月25日(月) 16:15 〜 18:00 201A (2F)

コンビーナ:*片山 郁夫(広島大学大学院理学研究科地球惑星システム学専攻)、岡本 敦(東北大学大学院環境科学研究科)、川本 竜彦(京都大学大学院理学研究科附属地球熱学研究施設)、座長:岡本 敦(東北大学大学院環境科学研究科)

17:00 〜 17:15

[SCG60-18] 分子動力学シミュレーションによる石英表面の水の構造および物理化学特性の解明

*石川 慧1佐久間 博2土屋 範芳1 (1.東北大学大学院環境科学研究科、2.独立行政法人 物質・材料研究機構)

キーワード:界面水, 石英, 分子動力学, 自己拡散係数

Structure of water in thin film may have different characteristics compared with that of bulk water. Thin film water can be present at mineral grain boundaries or fractures, and its structure might be influenced by mineral surface. In this study, classical molecular dynamics (MD) simulations were performed to investigate the structure and physico-chemical characteristics of thin film water on a quartz surface.
The model of the quartz surface was characterized by the termination of silanol (Si-OH) group. Water molecules were confined between these surfaces, and we simulated several thicknesses of water in the slab geometry.
Density of water oscillates to be about 1 nm from the quartz surface at 298 K. This structure became less clear with heating, and almost disappeared above 473 K. The self-diffusion coefficients of the confined water were calculated from mean square displacements. These values were lower than that of bulk water indicating that the mobility of confined water is low between quartz surfaces.
These changes in the physical properties of interfacial water on quartz might affect such as slips in the fracture surface of the Earth’s crust.