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    Surface electronic states of meteoritic nanodiamonds

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    Author
    Garvie, Laurence A. J.
    Buseck, Peter R.
    Issue Date
    2006-01-01
    Keywords
    carbonaceous chondrites
    electron microscopy
    aqueous alteration
    organic matter
    
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    Citation
    Garvie, L. A. J., & Buseck, P. R. (2006). Surface electronic states of meteoritic nanodiamonds. Meteoritics & Planetary Science, 41(5), 667-672.
    Publisher
    The Meteoritical Society
    Journal
    Meteoritics & Planetary Science
    URI
    http://hdl.handle.net/10150/656701
    DOI
    10.1111/j.1945-5100.2006.tb00982.x
    Additional Links
    https://meteoritical.org/
    Abstract
    The C K edge of Orgueil nanodiamonds (C-delta diamonds) was acquired by electron energy-loss spectroscopy (EELS), with an energy resolution of 300 meV. The spectra show peaks at 282.5, 284.7, and 286.4 eV, which occur in the band gap below the main diamond edge and are absent from the bulk diamond spectrum. These peaks are attributed to transitions from degrees C 1s surface core levels to unoccupied surface states, and arise from single and pi-bonded dangling bonds and C-H bonds. A shoulder to the main absorption edge at 287.8 eV may correspond to hydrocarbon adsorbates. These results can be used to further our understanding of C-delta diamond structure and may reveal the presence of a fullerene-like surface. The unique surface electronic states of the C-delta diamond surfaces are expected to affect their optical properties, which are dependent on features such as extent of H coverage, particle size, and surface structure.
    Type
    Article
    text
    Language
    en
    ISSN
    1945-5100
    ae974a485f413a2113503eed53cd6c53
    10.1111/j.1945-5100.2006.tb00982.x
    Scopus Count
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    Meteoritics & Planetary Science, Volume 41, Number 5 (2006)

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