Temperature of the inner-core boundary of the Earth: Melting of iron at high pressure from first-principles coexistence simulations

被引:127
|
作者
Alfe, Dario [1 ,2 ,3 ]
机构
[1] UCL, Dept Earth Sci, London WC1E 6BT, England
[2] UCL, Dept Phys & Astron, Mat Simulat Lab, London WC1E 6BT, England
[3] UCL, London Ctr Nanotechnol, London WC1E 6BT, England
来源
PHYSICAL REVIEW B | 2009年 / 79卷 / 06期
基金
英国工程与自然科学研究理事会;
关键词
density functional theory; Earth core; free energy; geology; high-pressure effects; iron; liquid metals; melting; AUGMENTED-WAVE METHOD; MOLECULAR-DYNAMICS; ALGORITHM; CURVE; CELL;
D O I
10.1103/PhysRevB.79.060101
中图分类号
T [工业技术];
学科分类号
08 ;
摘要
The Earth's core consists of a solid ball with a radius of 1221 Km, surrounded by a liquid shell which extends up to 3480 km from the center of the planet, roughly half way toward the surface (the mean radius of the Earth is 6373 km). The main constituent of the core is iron, and therefore the melting temperature of iron at the pressure encountered at the boundary between the solid and the liquid [the inner-core boundary (ICB)] provides an estimate of the temperature of the core. Here I report the melting temperature of Fe at pressures near that of the ICB, obtained with first-principles techniques based on density-functional theory. The calculations have been performed by directly simulating solid and liquid iron in coexistence and show that and at a pressure of similar to 328 GPa iron melts at similar to 6370 +/- 100 K. These findings are in good agreement with earlier simulations, which used exactly the same quantum-mechanics techniques but obtained melting properties from the calculation of the free energies of solid and liquid Fe.
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页数:4
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