Although precipitates’ compositions are theoretically determined by thermodynamics, their formation kinetics can also lead to composition variations that allow further structural evolution, making the precipitation path more complex.
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References
Orthacker, A. et al. Nat. Mater. https://doi.org/10.1038/s41563-018-0209-z (2018).
Forbord, B., Lefebvre, W., Danoix, F., Hallem, H. & Marthinsen, K. Scripta Mater. 51, 333–337 (2004).
Tolley, A., Radmilovic, V. & Dahmen, U. Scripta Mater. 52, 621–625 (2005).
Fuller, C. B., Murray, J. L. & Seidman, D. N. Acta Mater. 53, 5401–5413 (2005).
Clouet, E. et al. Nat. Mater. 5, 482–488 (2006).
Cahn, J. W. & Hilliard, J. E. J. Chem. Phys. 31, 688–699 (1959).
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Clouet, E. Excess solvent in precipitates. Nature Mater 17, 1060–1061 (2018). https://doi.org/10.1038/s41563-018-0224-0
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DOI: https://doi.org/10.1038/s41563-018-0224-0