Ab initio simulations of hot dense methane during shock experiments

被引:32
|
作者
Sherman, Benjamin L. [1 ]
Wilson, Hugh F. [2 ]
Weeraratne, Dayanthie [1 ]
Militzer, Burkhard [2 ,3 ]
机构
[1] Calif State Univ Northridge, Dept Geol Sci, Northridge, CA 91330 USA
[2] Univ Calif Berkeley, Dept Earth & Planetary Sci, Berkeley, CA 94720 USA
[3] Univ Calif Berkeley, Dept Astron, Berkeley, CA 94720 USA
基金
美国国家科学基金会; 美国国家航空航天局;
关键词
HIGH-PRESSURE; GIANT; HYDROCARBONS; HYDROGEN; INTERIOR; WATER; CORE; CH4;
D O I
10.1103/PhysRevB.86.224113
中图分类号
T [工业技术];
学科分类号
08 ;
摘要
Using density functional theory molecular dynamics simulations, we predict shock Hugoniot curves of precompressed methane up to 75 000 K for initial densities ranging from 0.35 to 0.70 g cm(-3). At 4000 K, we observe the transformation into a metallic, polymeric state consisting of long hydrocarbon chains. These chains persist when the sample is quenched to 300 K, leading to an increase in shock compression. At 6000 K, the sample transforms into a plasma composed of many, short-lived chemical species. We conclude by discussing implications for the interiors of Uranus and Neptune and analyzing the possibility of creating a superionic state of methane in high pressure experiments. DOI:10.1103/PhysRevB.86.224113
引用
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页数:8
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