日本地球惑星科学連合2022年大会

講演情報

[E] ポスター発表

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-IT19] 地球深部科学

2022年5月30日(月) 11:00 〜 13:00 オンラインポスターZoom会場 (22) (Ch.22)

コンビーナ:太田 健二(東京工業大学理学院地球惑星科学系)、コンビーナ:河合 研志(東京大学大学院理学系研究科地球惑星科学専攻)、飯塚 毅(東京大学)、コンビーナ:土屋 旬(愛媛大学地球深部ダイナミクス研究センター)、座長:太田 健二(東京工業大学理学院地球惑星科学系)、土屋 旬(愛媛大学地球深部ダイナミクス研究センター)、飯塚 毅(東京大学)、河合 研志(東京大学大学院理学系研究科地球惑星科学専攻)

11:00 〜 13:00

[SIT19-P03] Heat transport properties of the slab constituent minerals from first-principles

*出倉 春彦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:下部マントル、熱輸送特性、理論

The temperature structure of the Earth's interior is still one of the most uncertain physical quantities. Since viscosity is a key parameter controlling the style of the mantle convection and is sensitive to temperature, the temperature profile of the mantle provides a basis for a better understanding of mantle dynamics. The subducting slab is one of the potential sources producing both the temperature and chemical heterogeneities in the lower mantle. The heat transport mechanism by thermal conduction is likely dominant in the subducting slab. Therefore, the temperature heterogeneity of the deep mantle induced by the subduction can be better constrained by determining the lattice thermal conductivity (κ) of its constituent minerals. However, precise determinations of the κ under the deep mantle conditions are still challenging, making the heat transport properties of the subducting slab remain unclear. We have recently initiated the first-principles determination of the κ of those minerals based on the density-functional theory for a tighter constraint on the temperature structure. In this presentation, we will report our progress of both harmonic and anharmonic phonon calculations of SiO2 and CaSiO3 perovskite necessary to compute κ under the lower mantle conditions.