JpGU-AGU Joint Meeting 2017

講演情報

[EE] 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-IT22] [EE] 核-マントルの相互作用と共進化

2017年5月20日(土) 15:30 〜 17:00 A05 (東京ベイ幕張ホール)

コンビーナ:土屋 卓久(愛媛大学地球深部ダイナミクス研究センター)、寺崎 英紀(大阪大学大学院理学研究科)、Satish-Kumar Madhusoodhan(Department of Geology, Faculty of Science, Niigata University)、入舩 徹男(愛媛大学地球深部ダイナミクス研究センター)、Hernlund John(Earth-Life Science Institute, Tokyo Institute of Technology)、大谷 栄治(東北大学大学院理学研究科地学専攻)、座長:土屋 卓久(愛媛大学地球深部ダイナミクス研究センター)

15:30 〜 15:45

[SIT22-19] Effects of Fe and Al incorporations on MgSiO3 postperovskite phase boundary

★招待講演

*Xianlong Wang1,2Taku Tsuchiya3,4Zhi Zeng1,2 (1.Institute of Solid State Physics, Chinese Academy of Sciences、2.University of Science and Technology of China、3.Geodynamics Research Center, Ehime University、4.Earth-Life Science Institute, Tokyo Institute of Technology)

キーワード:First-principles method, internally consistent LSDA+U, MgSiO3, postperovskite

MgSiO3 bridgmanite (Br) will undergoes a post-perovskite (PPv) phase transition[1,2,3] in the pressure (P) and temperature (T) conditions corresponding to the Earth’s D” layer. Therefore, The phase change is recognized as the key for understanding the seismological observations in the D” layer. However, to date, it is still a challenging subject to determine the phase transition boundary preciously in the geophysically relevant Fe and Al-bearing compositions. Based on the first-principles methods combined with the internally consistent LSDA+U method and the lattice dynamics approach, the high-P,T thermodynamics of the MgSiO3 phases are directly calculated with incorporation of 6.25 mol% of Fe2+, Fe3+Fe3+, Fe3+Al3+, and Al3+Al3+ [4,5]. Using calculated free energies, we determine the PPv phase boundaries for Fe and Al-bearing compositions. Our results show that at 2500 K, incorporations of Fe3+Fe3+ and Fe3+Al3+ span coexisting domains between Br and PPv significantly with lowering the transition pressure, in contrast to the Fe2+ and Al3+Al3+-bearing cases.

References:
[1] M. Murakami, K. Hirose, K. Kawamura, N. Sata, and Y. Ohishi, Science 304, 855 (2004).
[2] A. Oganov, and S. Ono, Nature 430, 445 (2004).
[3] T. Tsuchiya, J. Tsuchiya, K. Umemoto, and R. M. Wentzcovitch, Earth. Planet. Sci. Lett. 224, 241 (2004).
[4] J. Tsuchiya, and T. Tsuchiya, Proc. Natl. Acad. Sci. USA 105, 19160 (2008).
[5] A. Metsue, and T. Tsuchiya, Geophys. J. Int. 190, 310 (2012).