日本地球惑星科学連合2016年大会

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インターナショナルセッション(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-IT07] Structure and dynamics of Earth and Planetary deep interiors

2016年5月22日(日) 13:45 〜 15:15 201B (2F)

コンビーナ:*芳野 極(岡山大学地球物質科学研究センター)、趙 大鵬(東北大学大学院理学研究科附属地震・噴火予知研究観測センター)、中川 貴司(海洋研究開発機構数理科学・先端技術研究分野)、座長:Kono Yoshio(Carnegie Institution for Science Washington)、亀山 真典(国立大学法人愛媛大学地球深部ダイナミクス研究センター)

15:00 〜 15:15

[SIT07-18] First-principles study of solid iron-hydrogen alloys under high pressure

*梅本 幸一郎1廣瀬 敬1 (1.東京工業大学地球生命研究所)

キーワード:Iron-hydrogen alloys, First principles, Crystal structure at high pressure

Hydrogen and iron are two of major constituents of the Earth and planetary interiors. The crystal structure of solid FeHx is one of the most fundamental information in order to understand properties of planetary cores. Recently, hydrogen-rich phases, FeH2 and FeH3, were experimentally synthesized [1]. The crystal structure of FeH3 was clarified by comparing experimental compression curve with calculated one. On the other hand, the structure of FeH2 remains unclear. It is mainly because the hydrogen positions are quite difficult to be determined by x-ray diffraction measurements. Ref. 1 proposed the crystal structure of FeH2, but it is less consistent with its experimental compression curve. Here we report the results of first-principles calculations on FeH2. We find the new hydrogen positions which lead to more stable structure than proposed by Ref. 1 and reproduces experimental compression curve very well. Our new structure will be essential for constraining the amount of hydrogen in iron alloys.
[1] C. M. Pépin, A. Dewaele, G. Geneste, P. Loubeyre, and M. Mezouar, Phys. Rev. Lett. 113, 265504 (2014).