Predicting the Stability of Fullerene Allotropes Throughout the Periodic Table
Author(s)
Ng, Stanley S. H.; Zhao, Qing; Kulik, Heather Janine
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We present a systematic, first-principles study of the role of elemental identity in determining electronic, energetic, and geometric properties of representative A₂₈B₂₈, A₃₀B₃₀, and A₃₆B₃₆ III–V (A = B, Al, Ga, or In and B = N, P, or As) and II–VI (A = Zn or Cd and B = S or Se) fullerene allotropes. A simple descriptor comprising electronegativity differences and covalent radii captures the relative fullerene stability with respect to a nanoparticle reference, and we demonstrate transferability to group IV A₇₂ (A = C, Si, or Ge) fullerenes. We identify the source of relative stability of the four- and six-membered-ring-containing A₃₆B₃₆ and A₂₈B₂₈ fullerene allotropes to the less stable, five-membered-ring-containing A₃₀B₃₀ allotrope. Relative energies of hydrogen-passivated single ring models explain why the even-membered ring structures are typically more stable than the A₃₀B₃₀ fullerene, despite analogies to the well-known C₆₀ allotrope. The ring strain penalty in the four-membered ring is comparable to or smaller than the nonpolar bond penalty in five-membered rings for some materials, and, more importantly, five-membered rings are more numerous in A₃₀B₃₀ than four-membered rings in A₃₆B₃₆ or A₂₈B₂₈ allotropes. Overall, we demonstrate a path forward for predicting the relative stability of fullerene allotropes and isomers of arbitrary shape, size, and elemental composition.
Date issued
2016-08Department
Massachusetts Institute of Technology. Department of Chemical Engineering; Massachusetts Institute of Technology. Department of Mechanical EngineeringJournal
Journal of Physical Chemistry C
Publisher
American Chemical Society (ACS)
Citation
Zhao, Qing; Ng, Stanley S. H. and Kulik, Heather J. “Predicting the Stability of Fullerene Allotropes Throughout the Periodic Table.” The Journal of Physical Chemistry C 120, no. 30 (August 2016): 17035–17045 © 2016 American Chemical Society
Version: Author's final manuscript
ISSN
1932-7447
1932-7455