Evidence for multiple liquid-liquid phase transitions in carbon, and the Friedel ordering of its liquid state

被引:3
|
作者
Dharma-wardana, M. W. C. [1 ]
Klug, Dennis D. [1 ]
机构
[1] Natl Res Council Canada, Ottawa, ON K1A 0R6, Canada
关键词
EQUATION-OF-STATE; TRANSPORT-PROPERTIES; ELECTRON-GAS; ION-ION; DENSE; PLASMA; GE;
D O I
10.1063/5.0077343
中图分类号
O35 [流体力学]; O53 [等离子体物理学];
学科分类号
070204 ; 080103 ; 080704 ;
摘要
Carbon, the fourth most abundant element in the universe, forms a metallic fluid with transient covalent bonds on melting. Its liquid-liquid phase transitions, intensely sought using simulations, had been elusive. Here, we use density functional theory (DFT) simulations with up to 108 atoms using molecular dynamics, as well as one-atom DFT as implemented in the neutral pseudo-atom method where multi-atom effects are treated by ion-ion correlation functionals. Both methods use electron-electron exchange correlation functionals for electron many-body effects. Here, we show using both methods that liquid carbon displays multiple liquid-liquid transitions linked to changes in coordination number in the density range 3-6 g/cm(3) when a coordination number of 12 is reached. The transitions disappear by 4 eV in temperature. The calculated pressures and transition densities are shown to be sensitive to the exchange-correlation functionals used. Significantly, we find that a simple metallic model yields the structure factors and thermodynamics with quantitative accuracy, without invoking any covalent-bonding features. The ion-ion structure factor for these densities and temperatures is found to have a subpeak tied to twice the Fermi wavevector, constraining the fluid in momentum space. The dominant Friedel oscillations forming the pair interactions correlate the ions and drive the multiple liquid-liquid phase transitions. Our results suggest that liquid carbon typifies a class of fluids whose structure is ordered by the long-ranged Friedel oscillations in the pair-potentials. These results are critical to terrestrial and astrophysical studies, inertial fusion using carbon drivers, refined shock experiments, and in seeking new carbon-based materials.
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页数:13
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