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-IT06] Interaction and Coevolution of the Core and Mantle

2016年5月23日(月) 15:30 〜 17:00 304 (3F)

コンビーナ:*田中 聡(海洋研究開発機構 地球深部ダイナミクス研究分野)、土屋 卓久(愛媛大学地球深部ダイナミクス研究センター)、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)、Satish-Kumar Madhusoodhan(Department of Geology, Faculty of Science, Niigata University)

16:45 〜 17:00

[SIT06-24] Electron-phonon contribution to electrical resistivity of hcp Fe

*出倉 春彦1土屋 卓久1 (1.愛媛大学地球深部ダイナミクス研究センター)

キーワード:Earth's core, Electron transport property, First-principles calculation

Determination of electron transport property of the Earth’s core is a key to understanding its thermal property. Electrical resistivity (ρ) of a solid metal comprises electron-phonon and electron-electron scattering mechanisms. Two recent first-principles studies however show a significant difference in the electron-phonon contribution (ρel-ph) of hcp Fe (M. Pozzo, C. Davies, D. Gubbins, and D. Alfe, Nature, 485, 355, 2012; P. Zhang, R. E. Cohen, and K. Haule, Nature, 517, 605, 2015). While Pozzo et al. reported ρel-ph smaller than the conventional estimates (e.g. F. D. Stacey and O. L. Anderson, Phys. Earth Planet Int, 124, 153, 2001), Zhang et al. showed approximately two times larger ρel-ph than Pozzo et al’s and closer to the conventional values. To aim for verifying these previous studies, we develop a technique to compute electron-phonon interaction and ρel-ph of metals based on the density-functional perturbation theory. In this talk, in addition to our technical advantage, preliminary results on the electrical resistivity of hcp Fe under high-P,T condition are presented.