日本地球惑星科学連合2018年大会

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] 核-マントルの相互作用と共進化

2018年5月23日(水) 10:45 〜 12:15 国際会議室(IC) (幕張メッセ国際会議場 2F)

コンビーナ:飯塚 毅(東京大学)、渋谷 秀敏(熊本大学大学院先端科学研究部基礎科学部門地球環境科学分野)、土屋 卓久(愛媛大学地球深部ダイナミクス研究センター、共同)、太田 健二(東京工業大学大学院理工学研究科地球惑星科学専攻)、座長:角野 浩史舘野 繁彦飯塚 毅

12:00 〜 12:15

[SIT22-24] Effects of light elements on transport properties of liquid Fe alloys under high pressure.

*大村 訓史1土屋 卓久2市川 浩樹3 (1.広島工業大学、2.愛媛大学、3.東京工業大学)

キーワード:電気伝導度、熱伝導度、液体鉄合金、高圧、第一原理分子動力学シミュレーション

It is believed that Earth’s outer core consists of liquid iron (or liquid-nickel alloy) with light element impurities. For understanding magnetic and thermal behaviors of the Earth, it is required to investigate electrical and thermal conductivities of liquid iron and influence of the light elements on these properties. Several experimental studies investigated the electrical and thermal conductivities under high pressure by shock compression experiments (Keeler, 1969 : Bi ,2002) and by experiments in a laser-heated diamond anvil cell ( Ohta, 2016 : Konôpková 2016). First principle calculations also have been used to investigate transport properties of liquid iron and mixtures with silicon and oxygen. (Pozzo, 2012, 2013 : de Koker, 2012)

Under this circumstance, we have investigated effects of light elements (including all candidate other than silicon and oxygen) on transport properties of liquid Fe alloy under high pressure by using ab initio molecular dynamics simulations. To provide further details of the effects of light-element, in addition to the type of light element, we have investigated how much transport properties are affected by the amount of light elements. This time, we discuss effects of the light element on transport properties of liquid Fe alloys in terms of the type and amount of light elements.

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)
Z. Konôpková et al., Nature 534 99 (2016)