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Ni and Co Incorporation in Forsterite: A Density Functional Theory Study with Hubbard Correction
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    Ni and Co Incorporation in Forsterite: A Density Functional Theory Study with Hubbard Correction
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    ACS Earth and Space Chemistry

    Cite this: ACS Earth Space Chem. 2024, 8, 5, 1027–1038
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    https://doi.org/10.1021/acsearthspacechem.3c00370
    Published April 17, 2024
    Copyright © 2024 American Chemical Society

    Abstract

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    Ni and Co are critical elements for the world economy and modern technologies. Mafic and ultramafic deposits represent low-grade yet abundant alternatives to traditional Ni and Co ores. In this work, density functional theory (DFT) with the Hubbard U correction (DFT+U) was used to simulate the incorporation of Ni and Co in forsterite (Mg2SiO4), the Mg endmember of olivine, a common mineral in mafic and ultramafic rocks. Hubbard U terms for Ni and Co were parametrized using a series of oxide, hydroxide, carbonate, silicate, and sulfide minerals relevant to extraction and recovery of Ni and Co from mafic and ultramafic deposits. Electronic, energetic, magnetic, and structural properties were considered in the parametrization. For each of Ni and Co, an effective Hubbard correction (Ueff) value that optimized agreement with either experimental data or a hybrid exchange-correlation functional for all of the minerals considered is reported. DFT+U ab initio molecular dynamics (AIMD) simulations of Ni and Co incorporated into the M1 and M2 octahedral sites of forsterite were then performed. Ni and Co substitution in the M1 site was more energetically favorable than substitution in the M2 site, in agreement with published partition coefficients. AIMD trajectories were used to compute extended X-ray absorption fine structure (EXAFS) spectra of Ni in the M1 and M2 sites for direct fitting to a published experimental spectrum of Ni in a natural San Carlos olivine sample. The results of the fit indicated that ordering of Ni in the M1 site was not as strong at the low Ni concentrations relevant to mafic and ultramafic silicate minerals as that at the higher concentrations of the Ni-Mg olivine solid solutions studied to date.

    Copyright © 2024 American Chemical Society

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    Supporting Information

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    The Supporting Information is available free of charge at https://pubs.acs.org/doi/10.1021/acsearthspacechem.3c00370.

    • Comparison of lattice parameters calculated with PBE0 and PBE0-D3, plots of density of states and tables summarizing the band gap energies, reaction enthalpies, magnetic moments, and structural details of the 18 Ni and Co phases considered in this work, plots of the root-mean-square absolute error for each property, plots of the instantaneous energy and average Ni–O bond lengths and their running averages for Ni in the M1 and M2 sites of forsterite, and Ni K-edge EXAFS spectra of Ni in the M1 and M2 sites of forsterite at 0 and 298 K (PDF)

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    Cited By

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    This article is cited by 1 publications.

    1. Arianna M. Morfin, C. Heath Stanfield, Madeline A. Murchland, Madeline F. Bartels, Alexandra B. Nagurney, Quin R.S. Miller, H. Todd Schaef. Structure–Composition Relationships for Mg–Ni and Mg–Fe Olivine. ACS Earth and Space Chemistry 2024, 8 (9) , 1713-1724. https://doi.org/10.1021/acsearthspacechem.4c00044

    ACS Earth and Space Chemistry

    Cite this: ACS Earth Space Chem. 2024, 8, 5, 1027–1038
    Click to copy citationCitation copied!
    https://doi.org/10.1021/acsearthspacechem.3c00370
    Published April 17, 2024
    Copyright © 2024 American Chemical Society

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