日本地球惑星科学連合2018年大会

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[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) 09:00 〜 10:30 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:河合 研志飯塚 理子

09:00 〜 09:15

[SIT22-13] Phonon energies and lifetimes of MgO at high temperature: Implications for thermal conductivity

★Invited Papers

*Daniele Antonangeli1 (1.Sorbonne Université - CNRS - IMPMC)

キーワード:anharmonicity, thermal conductivity, MgO, high temperature, lower mantle

Thermal conductivity is a fundamental physical parameter that largely controls the heat transfer in Earth’s interior. Despite its importance, the thermal conductivity of mantle minerals is one of the least constrained properties at high pressure (P) and high temperature (T) as direct measurements at pertinent P-T conditions remains a technical challenge. Current geophysical models rely on the extrapolations of low P data and, increasingly so, on results from ab initio calculations. However, the validity and versatility of the various theoretical approaches used in literature remain to be tested again experiments. The direct measurements of vibrational and anharmonic properties such as phonon energy and linewidth (inverse of lifetime) as a function of P and T provide the most straightforward benchmark for the theoretical calculations as these are the key parameters entering the Boltzmann transport equation used to calculate lattice thermal conductivity.

Here I present the determination of phonon energies and phonon widths of single crystalline MgO as function of temperature, by inelastic x-ray scattering up to 1220 K, and by infrared reflectivity up to 1400 K. Measurements are complemented by density functional theory calculations. The comparison of experimental and computational results allows assessing the theoretical phonon-phonon scattering coefficients and to estimate the relative weight of intrinsic and extrinsic phonon scattering mechanisms.