日本地球惑星科学連合2022年大会

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[E] 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-IT17] 地球型惑星内部での液体の特性とその役割

2022年5月22日(日) 13:45 〜 15:15 102 (幕張メッセ国際会議場)

コンビーナ:坂巻 竜也(東北大学大学院理学研究科)、コンビーナ:中島 陽一(熊本大学大学院先導機構)、座長:坂巻 竜也(東北大学大学院理学研究科)、中島 陽一(熊本大学大学院先導機構)

14:05 〜 14:20

[SIT17-02] Pressure-induced structural change of liquid sulfur from polymeric liquid to simple liquid

*Satoshi Ohmura1 (1.Hiroshima Institute of Technology)

Liquid sulfur near the melting temperature of 388 K consists of S8 ring molecules. With increasing temperature, a structural transition from molecular liquid to chain polymeric liquid occurs. For high pressure conditions, some experimental and theoretical studies have been reported [Brazhkin 1991; Zhao, 2014; Liu, 2014; Plašienka, 2015] for structural changes in liquid sulfur from long-chain to short-chain structures under high pressure up to 15.8 GPa. However, structural properties under further high pressure (i.e., structures that reach beyond a chain structure) have not been discussed. For this reason, in this study, we have investigated the structural properties of liquid sulfur under high pressures up to approximately 500 GPa by means of ab initio molecular dynamics simulations. From our simulations, it is found that the liquid sulfur has a covalent-like interactions even in metallic state, and liquid sulfur has a simple liquid structure at 320 GPa and higher pressures (Ohmura, 2019). In this study, we will also discuss the similarities of pressure-induced structural change in other liquid chalcogens[Shimojo, 2003; Ohmura, 2011].