English

Direct MD simulation of liquid-solid phase equilibria for two-component plasmas

Solar and Stellar Astrophysics 2012-07-05 v2 Plasma Physics

Abstract

We determine the liquid-solid phase diagram for carbon-oxygen and oxygen-selenium plasma mixtures using two-phase MD simulations. We identified liquid, solid, and interface regions using a bond angle metric. To study finite size effects, we perform 27648 and 55296 ion simulations. To help monitor non-equilibrium effects, we calculate diffusion constants DiD_i. For the carbon-oxygen system we find that DOD_O for oxygen ions in the solid is much smaller than DCD_C for carbon ions and that both diffusion constants are 80 or more times smaller than diffusion constants in the liquid phase. There is excellent agreement between our carbon-oxygen phase diagram and that predicted by Medin and Cumming. This suggests that errors from finite size and non-equilibrium effects are small and that the carbon-oxygen phase diagram is now accurately known. The oxygen-selenium system is a simple two-component model for more complex rapid proton capture nucleosynthesis ash compositions for an accreting neutron star. Diffusion of oxygen, in a predominately selenium crystal, is remarkably fast, comparable to diffusion in the liquid phase. We find a somewhat lower melting temperature for the oxygen-selenium system than that predicted by Medin and Cumming. This is probably because of electron screening effects.

Keywords

Cite

@article{arxiv.1108.3101,
  title  = {Direct MD simulation of liquid-solid phase equilibria for two-component plasmas},
  author = {A. S. Schneider and J. Hughto and C. J. Horowitz and D. K. Berry},
  journal= {arXiv preprint arXiv:1108.3101},
  year   = {2012}
}

Comments

18 pages, 32 figures, submitted to Phys. Rev. E, added substantial new results for oxygen-selenium system

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