Collision-induced fusion of two C60 fullerenes: Quantum chemical molecular dynamics simulations

Jacek Jakowski, Stephan Irle, and Keiji Morokuma
Phys. Rev. B 82, 125443 – Published 24 September 2010

Abstract

We characterize the collision-induced fusion reaction of buckminsterfullerenes by means of direct self-consistent-charge density-functional tight-binding molecular dynamics simulations. In agreement with experimental data, we find that the highest probability of fusion is for collisions with incident energy range of 120–140 eV. In this energy region, fusion occurs by way of the formation of hot, vibrationally excited peanut-shaped structures within 1 ps. These nanopeanuts further undergo relaxation to short carbon nanotubes and are cooling by evaporation of short carbon chains during the next 200 ps. The size of the fusion product after the evaporation agrees well with the average size of carbon clusters experimentally detected after collisions on the microsecond time scale. The average number of sp3 carbons in our simulations is in an excellent correlation with experimental cross sections.

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  • Received 27 April 2010

DOI:https://doi.org/10.1103/PhysRevB.82.125443

©2010 American Physical Society

Authors & Affiliations

Jacek Jakowski*

  • National Institute for Computational Sciences, JICS-ORNL, One Bethel Valley Road, Bldg 5100 ms 6173, Oak Ridge, Tennessee 37831, USA and Cherry L. Emerson Center for Scientific Computation and Department of Chemistry, Emory University, 1515 Dickey Drive, Atlanta, Georgia 30322, USA

Stephan Irle

  • Institute for Advanced Research and Department of Chemistry, Nagoya University, Nagoya 464-8602, Japan

Keiji Morokuma

  • Cherry L. Emerson Center for Scientific Computation and Department of Chemistry, Emory University, 1515 Dickey Drive, Atlanta, Georgisa 30322, USA and Fukui Institute for Fundamental Chemistry, Kyoto University, Sakyo, Kyoto 6006-8103, Japan

  • *jacek@euch4e.chem.emory.edu
  • sirle@iar.nagoya-u.ac.jp
  • morokuma@euch4e.chem.emory.edu

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Issue

Vol. 82, Iss. 12 — 15 September 2010

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