典型文献
Partially Diffusive Helium-Silica Compound under High Pressure
文献摘要：
Helium is the second most abundant element in the universe,and together with silica,they are important components of giant planets.Exploring the reactivity and state of helium and silica under high pressure is crucial for understanding of the evolution and internal structure of giant planets.Here,using first-principles calculations and crystal structure predictions,we identify four stable phases of a helium-silica compound with seven/eight-coordinated silicon atoms at pressure of 600-4000 GPa,corresponding to the interior condition of the outer planets in the solar system.The density of HeSiO2 agrees with current structure models of the planets.This helium-silica compound exhibits a superionic-like helium diffusive state under the high-pressure and high-temperature conditions along the isentropes of Saturn,a metallic fluid state in Jupiter,and a solid state in the deep interiors of Uranus and Neptune.These results show that helium may affect the erosion of the rocky core in giant planets and may help to form a diluted core region,which not only highlight the reactivity of helium under high pressure but also provide evidence helpful for building more sophisticated interior models of giant planets.
文献关键词：
中图分类号：
作者姓名：
Cong Liu;Junjie Wang;Xin Deng;Xiaomeng Wang;Chris J.Pickard;Ravit Helled;Zhongqing Wu;Hui-Tian Wang;Dingyu Xing;Jian Sun
作者机构：
National Laboratory of Solid State Microstructures,School of Physics and Collaborative Innovation Center of Advanced Microstructures,Nanjing University,Nanjing 210093,China;Departament de Física,Universitat Politècnica de Catalunya,Campus Nord B4-B5,E-08034 Barcelona,Spain;Laboratory of Seismology and Physics of Earth's Interior,School of Earth and Space Sciences,University of Science and Technology of China,Hefei 230026,China;Department of Materials Science&Metallurgy,University of Cambridge,Cambridge CB3 0FS,UK;Advanced Institute for Materials Research,Tohoku University,Sendai 980-8577,Japan;Institute for Computational Science,Center for Theoretical Astrophysics&Cosmology,University of Zurich,Switzerland
文献出处：
引用格式：
[1]Cong Liu;Junjie Wang;Xin Deng;Xiaomeng Wang;Chris J.Pickard;Ravit Helled;Zhongqing Wu;Hui-Tian Wang;Dingyu Xing;Jian Sun-.Partially Diffusive Helium-Silica Compound under High Pressure)[J].中国物理快报（英文版）,2022(07):52-66
A类：
HeSiO2,isentropes,Saturn,Uranus
B类：
Partially,Diffusive,Helium,Silica,Compound,High,Pressure,second,most,abundant,element,universe,together,silica,they,are,important,components,giant,planets,Exploring,reactivity,state,helium,pressure,crucial,understanding,evolution,internal,structure,Here,using,first,principles,calculations,crystal,predictions,we,identify,four,stable,phases,compound,seven,eight,coordinated,silicon,atoms,GPa,corresponding,outer,solar,system,density,agrees,current,models,This,exhibits,superionic,like,diffusive,temperature,conditions,along,metallic,fluid,Jupiter,solid,deep,interiors,Neptune,These,results,show,that,may,affect,erosion,rocky,core,form,diluted,region,which,not,only,highlight,but,also,provide,evidence,helpful,building,more,sophisticated
AB值：
0.565119
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机标中图分类号，由域田数据科技根据网络公开资料自动分析生成，仅供学习研究参考。
