日本地球惑星科学連合2022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-IT19] 地球深部科学

2022年5月22日(日) 15:30 〜 17:00 展示場特設会場 (2) (幕張メッセ国際展示場)

コンビーナ:太田 健二(東京工業大学理学院地球惑星科学系)、コンビーナ:河合 研志(東京大学大学院理学系研究科地球惑星科学専攻)、飯塚 毅(東京大学)、コンビーナ:土屋 旬(愛媛大学地球深部ダイナミクス研究センター)、座長:飯塚 毅(東京大学)、河合 研志(東京大学大学院理学系研究科地球惑星科学専攻)

16:00 〜 16:15

[SIT19-09] Water partitioning between liquid metal and molten silicate under high pressure and temperature

*土屋 卓久1、大場 篤郎1 (1.愛媛大学地球深部ダイナミクス研究センター)

キーワード:第一原理自由エネルギー計算、熱力学積分法、水の金属-ケイ酸塩間分配

Metal/silicate water partitioning under high pressure is important to understand the water circulation in Earth's deep interior. Several srudies have therefore been conducted both experimentally and theoretically. However, primarily due to the technical difficulty in quantitative analyses of hydrogen, the reported experimental resuts scatter largely. Recent theoretical studies, on the other hand, suggest a siderophile behavior of hydrogen under high pressure, but those assume a simple molecular exchange reaction only and the stability of an experimentally suggested redox reaction is yet to be investigated. Therefore, the nature of metal/silicate partition reaction of water under high pressure remains largely unclear. In this study, we perform the ab initio free energy calculations based on the density functional theory and the thermodynamic integration method and predict reaction energy related to the high-pressure water partitioning between liquid iron and silicate melt with several different compositions considering both molecular exchange and redox reactions.