日本地球惑星科学連合2016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-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)

16:15 〜 16:30

[SIT06-22] 鉄と鉄-炭素合金の高温高圧弾性特性

*土屋 卓久1桑山 靖弘1石井 水晶3河合 研志2 (1.愛媛大学地球深部ダイナミクス研究センター、2.東京大学、3.ハーバード大学)

キーワード:内核、第一原理計算、弾性特性

Earth’s inner core (329~364 GPa and 5000~6000 K) is thought to be composed of solid Fe-Ni alloy with some light elements. Thermoelasticity of iron and iron-light element alloys is therefore a key to interpreting seismological information of the inner core: density, seismic wave velocities, and their anisotropy. However, several studies reported that pure hcp iron has a shear modulus distinctly larger than that of the inner core (e.g., Mao et al., 1998; Vocadlo et al., 2009). This large Poisson ratio of the inner core is one of the remaining inexplicable features of the deep Earth, and some studies recently proposed this be explained by alloyed with carbon (e.g., Chen et al., 2014).

In this study, we perform ab initio molecular dynamics simulations of iron and iron-carbon alloy. Also computations are conducted in a wide P,T range including, but not limited to, the inner core conditions to clarify the P,T effects on their elasticity more comprehensively, and to provide an internally-consistent thermoelastic model. In addition to checking the validity of the Birch’s law, the obtained Poisson ratio and aggregate anisotropy, with and without the pre-melting effect, are compared against seismological constraints to reinvestigate the viability of iron and iron-carbon alloy in the inner core.

Research supported by KAKENHI and the X-ray Free Electron Laser Priority Strategy Program (MEXT).