首页> 外文期刊>Geochimica et Cosmochimica Acta: Journal of the Geochemical Society and the Meteoritical Society >Near-surface controls on the composition of growing crystals: Car-Parrinello molecular dynamics (CPMD) simulations of Ti energetics and diffusion in alpha quartz
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Near-surface controls on the composition of growing crystals: Car-Parrinello molecular dynamics (CPMD) simulations of Ti energetics and diffusion in alpha quartz

机译:生长晶体组成的近表面控制:Ti能量学和α石英中扩散的Car-Parrinello分子动力学(CPMD)模拟

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Ab initio molecular dynamics simulations were used to explore changes in the vacancy-formation energy for Ti atoms and Ti-O bond characteristics in the outermost monolayers of the (100) and (010) prism faces of a quartz. Within 2 or 3 polyhedral layers of the crystal surface, the Ti vacancy-formation energy is substantially smaller than the bulk-lattice value of 11.8 eV. This is true of both oxygen-terminated surfaces and the geologically more realistic case in which the outermost oxygens are bonded to hydrogen. A key additional finding is that the Ti vacancy-formation energy near the H-terminated (100) surface differs by 1-2 eV from that near the H-terminated (010) surface. This difference means that the energy change accompanying Ti MSi exchange between the bulk lattice and the near surface is also different for (100) and (010). Ultimately, therefore, the equilibrium concentrations of Ti near these two prism faces will not be the same. During crystal growth, this compositional difference may be "captured" by the quartz lattice and preserved as sectoral variation in Ti content-a feature commonly observed in both synthetic and natural a quartz. In this respect, the MD simulations provide direct support for the growth entrapment model (GEM; Watson, 2004) for non-equilibrium uptake of trace elements. To complement the vacancy-formation energy results, we used the first-principles metadynamics method to calculate diffusion pathways and free energy barriers for Ti diffusion in the bulk a quartz lattice and in the near-surface region. The computed estimate of the bulk-lattice activation energy compares favorably with the experimentally determined value of 2.8 eV (Cherniak et al., 2007), lending credence to the method. Diffusion results for the near-surface reveal a steep decrease in the activation energy for Ti diffusion approaching the surface in the outermost 2-3 polyhedral layers of the crystal. This finding implies depth-dependent Ti diffusion in the near-surface (~0.5 nm), which is also a key aspect of the growth-entrapment model. Although our results are strictly applicable only to Ti in a quartz, the demonstration that impurity atom energetics and diffusion are functions of depth in the near-surface regionmay be broadly applicable, given the similarity in measured length scale of the near-surface relaxed region in a wide variety of minerals. Kinetic models of impurity uptake that do not consider these factors may be incomplete.
机译:从头开始进行分子动力学模拟,以探索石英(100)和(010)棱镜面最外层中Ti原子的空位形成能和Ti-O键特征的变化。在晶体表面的2或3个多面体层中,Ti空位形成能显着小于11.8 eV的体晶格值。对于以氧为末端的表面和在地质上更现实的情况(在此情况下,最外面的氧都与氢键合)都是如此。另一个重要的发现是,H端(100)表面附近的Ti空位形成能与H端(010)表面附近的Ti空位形成能相差1-2 eV。这种差异意味着对于(100)和(010),伴随在体晶格和近表面之间进行Ti MSi交换的能量变化也不同。因此,最终,这两个棱镜面附近的Ti的平衡浓度将不同。在晶体生长过程中,这种成分差异可能被石英晶格“捕获”,并保留为Ti含量的扇区变化-这是合成石英和天然石英中常见的特征。在这方面,MD模拟为痕量元素非平衡吸收的生长捕获模型(GEM; Watson,2004)提供了直接支持。为了补充空位形成能的结果,我们使用了第一性原理的元动力学方法来计算Ti扩散在整个石英晶格和近表面区域中的扩散途径和自由能垒。计算得出的晶格活化能估计值与实验确定的2.8 eV值相比具有优势(Cherniak等,2007),为该方法提供了依据。近表面的扩散结果表明,在晶体的最外面的2-3个多面体层中,Ti扩散接近表面的活化能急剧下降。这一发现暗示在近表面(〜0.5 nm)中深度依赖的钛扩散,这也是生长诱捕模型的关键方面。尽管我们的结果仅严格适用于石英中的Ti,但考虑到近表面弛豫区域的测量长度尺度相似,表明杂质原子的能量和扩散是近表面区域深度的函数的证明可能会广泛适用。多种矿物质。不考虑这些因素的杂质吸收动力学模型可能是不完整的。

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