水とアンモニアの超イオン状態と金属状態は,巨大惑星の条件下で発生する

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Updated: Oct 26, 2026

Analyzing Melts and Fluids from Ab Initio Molecular Dynamics Simulations with the UMD Package
06:37

Analyzing Melts and Fluids from Ab Initio Molecular Dynamics Simulations with the UMD Package

Published on: September 17, 2021

C Cavazzoni1, G L Chiarotti, S Scandolo

  • 1Istituto Nazionale per la Fisica della Materia (INFM) and International School for Advanced Studies (SISSA), Via Beirut 4, I-34014 Trieste, Italy.

Science (New York, N.Y.)
|January 5, 1999
PubMed
まとめ

シミュレーションにより,水とアンモニアが極端な圧力と温度下での新しい相を明らかにし,これは海王星と天王星を理解するために不可欠です. これらの発見は,絶縁性流体から金属状態と超離子固体相への移行を詳細に説明しています.

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