日本地球惑星科学連合2014年大会

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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-IT03_29AM2] Structure and dynamics of Earth and Planetary deep interiors

2014年4月29日(火) 11:00 〜 12:45 418 (4F)

コンビーナ:*田中 聡(海洋研究開発機構 地球内部ダイナミクス領域)、芳野 極(岡山大学地球物質科学研究センター)、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)、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)、ヘルンランド ジョン(東京工業大学 地球生命研究所)、座長: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)、竹内 希(東京大学地震研究所)

12:15 〜 12:30

[SIT03-13] A pyrolitic lower mantle with (Mg,Fe3+)(Si,Al3+)O3 perovskite

*WANG Xianlong1TSUCHIYA Taku1 (1.GRC, Ehime University and ELSI, Tokyo Institute of Technology)

キーワード:First-principles method, Internally consistent LSDA+U, Perovskite, Thermodynamic properties, Pyrolite

To better understand the Earth,s lower mantle (LM), thermodynamic properties (TDPs) of LM minerals with Fe and Al dopant should be illustrated more clearly. We have so far reported the TDPs of Fe-bearing MgO, MgSiO3 perovskite (Pv) and post perovskite. [1-4] We furthermore study the TDPs of Fe- and Al-bearing Pv, where the internally consistent LSDA+U method and the lattice dynamics method are applied. Two spin states, high (HS) and low spin state, two substitution sites, Mg and Si site, and several possible distribution configurations are considered. In the LM pressure range, HS Fe3+ substituted at the Mg site with Al3+ at the adjacent Si site (Fe-Al pair) is the most stable configuration and tends to distribute homogeneously in LM. Furthermore, negative frequency cannot be observed in the Fe-Al pair-bearing Pv, and Al contributes to middle frequency while Fe mainly to low part due to its heavy mass. This indicates that the Fe-Al pair is vibrationally stable. Incorporation of the pair for geophysically relevant concentrations can increase volume of Pv a little and has marginal effects on the TDPs of Pv except for thermal expansivity and Gruneisen parameter. Simulated densities, adiabatic bulk moduli ,and bulk sound velocities show that a composition close to pyrolite is accountable for the reference Earth model.References:[1] A. Metsue, and T. Tsuchiya, J. Geophys. Res. 116, B08207 (2011).[2] A. Metsue, and T. Tsuchiya, Geophys. J. Int. 190, 310 (2012).[3] H. Fukui, T. Tsuchiya, and A. Q. R. Baron, J. Geophys. Res. 117, B12202 (2012).[4] T. Tsuchiya, and X. Wang, J. Geophys. 118, 83 (2013).