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21日(日) 09:00 〜 10:30 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:大谷 栄治(東北大学大学院理学研究科地学専攻)

09:45 〜 10:00

[SIT22-28] Effects of light-element impurities on transport properties of liquid Fe-Ni alloy at Earth's core conditions

*大村 訓史1土屋 卓久2市川 浩樹2 (1.広島工業大学、2.愛媛大学)

キーワード:Ab initio molecular dynamics simulation, Transport properties, Liquid Fe-Ni mixtures

It is widely believed that the Earth's outer core consists of liqud iron (or liquid-nickel alloy) with light element impurities. Therefore, electrical and thermal conductivities of liquid iron-nickel alloys are important to understand magnetic and thermal behaviors of Earth.
Several experimental studies investigated the electrical conductivity or resistivity for iron under high pressure (Keeler, 1969 : Bi ,2002 : Ohta, 2016). Also, by using first principles calculations, electrical conductivity for liquid iron and mixtures with silicon and oxygen under high pressure has been investigated. (Pozzo, 2012, 2013 : de Koker, 2012)
Although first principles studies for liquid iron-oxygen and -silicon mixtures have been conducted so far, mixtures with other light elements such as hydrogen and carbon have not been investigated yet. Under this circumstance, in this study, we perform ab initio molecular dynamics simulations for liquid Fe-Ni alloy with H, C, O, S and Si. We calculate electronic and thermal conductivities at Earth's core conditions with using Kubo-Greenwood formulation. By comparing against results of pure system, we discuss effects of light element impurities on transport properties of liquid Fe-Ni alloy.



Reference
R.N. keeler and A.C. Mitchell, Solid state Commum. 7, 271 (1969)
Y. Bi, et al., J. Phys. Condens Matter 14, 10849 (2002)
M. Pozzo, et al., Nature 485, 355 (2012)
N de Koker, et al., Proc. Natl,. Acad. Sci. 109 4070 (2012)
M. Pozzo, et al., Phys. Rev. B 87 014110 (2013)
K. Ohta et al., Nature 534 95 (2016)