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      A classical view on nonclassical nucleation

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          Abstract

          <p id="d5629603e446">Nucleation is the process by which constituent building blocks first assemble to form a new substance. In the case of mineral formation from initially free ions in solution, the emergence of intermediary phases often determines the thermodynamics and kinetics of formation for the most stable phase. Our work on CaCO <sub>3</sub> mineralization reevaluates a topic of intense discussion: Can nucleation be explained by theories established over a century ago, or should new physical concepts, as recently proposed, be adopted? Our data show that classical theories can indeed be used to describe complex mechanisms of crystallization. In addition, we provide information about the properties of intermediate phases, which will aid in the design of additives to control mineralization. </p><p class="first" id="d5629603e452">Understanding and controlling nucleation is important for many crystallization applications. Calcium carbonate (CaCO <sub>3</sub>) is often used as a model system to investigate nucleation mechanisms. Despite its great importance in geology, biology, and many industrial applications, CaCO <sub>3</sub> nucleation is still a topic of intense discussion, with new pathways for its growth from ions in solution proposed in recent years. These new pathways include the so-called nonclassical nucleation mechanism via the assembly of thermodynamically stable prenucleation clusters, as well as the formation of a dense liquid precursor phase via liquid–liquid phase separation. Here, we present results from a combined experimental and computational investigation on the precipitation of CaCO <sub>3</sub> in dilute aqueous solutions. We propose that a dense liquid phase (containing 4–7 H <sub>2</sub>O per CaCO <sub>3</sub> unit) forms in supersaturated solutions through the association of ions and ion pairs without significant participation of larger ion clusters. This liquid acts as the precursor for the formation of solid CaCO <sub>3</sub> in the form of vaterite, which grows via a net transfer of ions from solution according to <i>z</i> Ca <sup>2+</sup> + <i>z</i> CO <sub>3</sub> <sup>2−</sup> → <i>z</i> CaCO <sub>3</sub>. The results show that all steps in this process can be explained according to classical concepts of crystal nucleation and growth, and that long-standing physical concepts of nucleation can describe multistep, multiphase growth mechanisms. </p>

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          The kinetics of precipitation from supersaturated solid solutions

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            Stable prenucleation calcium carbonate clusters.

            Calcium carbonate forms scales, geological deposits, biominerals, and ocean sediments. Huge amounts of carbon dioxide are retained as carbonate ions, and calcium ions represent a major contribution to water hardness. Despite its relevance, little is known about the precipitation mechanism of calcium carbonate, and specified complex crystal structures challenge the classical view on nucleation considering the formation of metastable ion clusters. We demonstrate that dissolved calcium carbonate in fact contains stable prenucleation ion clusters forming even in undersaturated solution. The cluster formation can be characterized by means of equilibrium thermodynamics, applying a multiple-binding model, which allows for structural preformation. Stable clusters are the relevant species in calcium carbonate nucleation. Such mechanisms may also be important for the crystallization of other minerals.
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              Late stages of spinodal decomposition in binary mixtures

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                Author and article information

                Journal
                Proceedings of the National Academy of Sciences
                Proc Natl Acad Sci USA
                Proceedings of the National Academy of Sciences
                0027-8424
                1091-6490
                September 19 2017
                September 19 2017
                : 114
                : 38
                : E7882-E7890
                Article
                10.1073/pnas.1700342114
                5617248
                28874584
                644553f7-7096-4323-ac84-f60a004e4ddb
                © 2017

                http://www.pnas.org/site/misc/userlicense.xhtml

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