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[MIS07-05] Numerical method for growth and dissolution processes of stoichiometric mineral crystals based on a phase-field model
Keywords:Crystal growth, Numerical simulation, Stoichiometric compound
In this study, we propose a numerical method for growth and melting of stoichiometric silicate compounds based on a phase-field (PF) model. We consider a binary system composed of two end members, A and B, with a crystal phase composed of only component A and a liquid phase assumed as a regular solution. We reformulated a binary PF model proposed by Kim et al. [3] in order to deal with a stoichiometric compound. We adopted a forsterite-SiO2 system and gave the free energy as functions of composition and temperature so as to agree with the phase diagram obtained experimentally [4]. We combined the free energy with the reformulated PF equations and carried out the numerical calculations in one-dimensional plane-parallel geometry.
First, we examined cases of diffusion-limited growth. With supercooled initial conditions, the incompatible component B was removed from the growing crystal to form the boundary layer. The liquid composition at the crystal-liquid interface was almost equal to the equilibrium value. Finally, the crystal growth ceased when the liquid composition reached equilibrium homogeneously. The growth rate was inversely proportional to the square of the elapsed time, which is consistent with the diffusion-limited condition. With under cooled initial conditions, the crystal melted to reach equilibrium like growth conditions. Second, we examined cases of kinetic-controlled growth. The growth rate is proportional to the driving force of crystal growth. In all calculations stated above the total free energy was monotonically decreased with time, which is consistent with the second law of thermodynamics.
The PF method can treat any systems if the free energy is formulated. Since some thermodynamics databases are available in silicate system (e.g., MELTS), our numerical method that can treat a stoichiometric compound enables us to investigate various situations considered in Earth and planetary science. In the future, we will extend our model to ternary or more system.
References: [1] W. W. Mullins and R. F. Sekerka, 1964, J. Appl. Phys. 35, 444. [2] D. Baker, 2008, Cont. Miner. Petro. 156, 377. [3] S. G. Kim et al., 1999, Phys. Rev. E 60, 7187. [4] N. L. Bowen and O. Andersen, 1914, 37, 487.