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Surface electronic states of meteoritic nanodiamonds
Author(s) -
GARVIE A. J. Laurence
Publication year - 2006
Publication title -
meteoritics and planetary science
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 1.09
H-Index - 100
eISSN - 1945-5100
pISSN - 1086-9379
DOI - 10.1111/j.1945-5100.2006.tb00982.x
Subject(s) - diamond , dangling bond , surface states , spectral line , electron energy loss spectroscopy , material properties of diamond , absorption spectroscopy , materials science , electronic structure , absorption (acoustics) , enhanced data rates for gsm evolution , spectroscopy , absorption edge , band gap , surface (topology) , chemical physics , chemistry , nanotechnology , silicon , computational chemistry , physics , optics , geometry , optoelectronics , transmission electron microscopy , computer science , composite material , telecommunications , quantum mechanics , astronomy , mathematics
— The C K edge of Orgueil nanodiamonds (Cδ 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 C 1s surface core levels to unoccupied surface states, and arise from single and π‐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 Cδ diamond structure and may reveal the presence of a fullerene‐like surface. The unique surface electronic states of the Cδ 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.