日本地球惑星科学連合2019年大会

講演情報

[E] 口頭発表

セッション記号 S (固体地球科学) » S-IT 地球内部科学・地球惑星テクトニクス

[S-IT20] 地球型惑星内部での液体の特性とその役割

2019年5月26日(日) 10:45 〜 12:15 A09 (東京ベイ幕張ホール)

コンビーナ:坂巻 竜也(東北大学大学院理学研究科)、中島 陽一(熊本大学大学院先導機構)、座長:坂巻 竜也(東北大学)、中島 陽一(熊本大学)

11:30 〜 12:00

[SIT20-03] Ab initio molecular dynamics study of atomic diffusion in covalent liquid under high pressure

★Invited Papers

*大村 訓史1土屋 卓久2 (1.広島工業大学、2.愛媛大学)

キーワード:液体、シリケート (ケイ酸塩)、原子拡散、第一原理分子動力学法

Transport properties of covalent liquids under high pressure are very interesting in the sense that they show unexpected pressure dependence. For a number of covalent liquids, such as SiO2, B2O3 and silicates abnormal behavior of the viscosity has been observed, i.e. the viscosity significantly drops with increasing pressure [1, 2, 3]. This anomalous behavior of the viscosity is considered to be related to the atomic diffusion in the liquids under pressure. It is, however, unclear how the rearrangement process of the covalent bonds is affected by compression. In order to explore the pressure dependence of microscopic diffusion mechanism in covalent liquids, we performed ab initio molecular dynamics simulations for liquid B2O3 and liquid basaltic aluminosilicate. These liquids has diffusivity maximum (viscosity minimum) under high pressure. We investigate the microscopic diffusion mechanism under high pressure. In the presentation, we discuss the origin of the anomalous pressure response of diffusivity from microscopic point of view.



[1] P. F. McMillan and M. C. Wildind. J. Non-Cryst. Solids, 355, 722
[2] V. Brazhkin, et al., Phys. Rev. Lett. 105, 115701 (2010)
[3] T. Sakamaki, et al., Nature Geoscience 6, 1041 (2013)