Ab initio infrared vibrational modes for neutral and charged small fullerenes (C 20 , C 24 , C 26 , C 28 , C 30 and C 60 )

Author:

Adjizian Jean-Joseph1ORCID,Vlandas Alexis2ORCID,Rio Jeremy3,Charlier Jean-Christophe1ORCID,Ewels Chris P.3ORCID

Affiliation:

1. Institute of Condensed Matter and Nanosciences, Université Catholique de Louvain, Chemin des Étoiles 8, 1348 Louvain-la-Neuve, Belgium

2. BioMEMS, Université Lille, CNRS, ISEN, UMR 8520-IEMN, 59000 Lille, France

3. Institut des Materiaux Jean Rouxel, CNRS, University of Nantes, UMR6502, 2 Rue de la Houssiniere, BP32229, 44322 Nantes Cedex 3, France

Abstract

We calculate the infrared (IR) absorption spectra using DFT B3LYP(6–311G) for a range of small closed-cage fullerenes, C n , n =20, 24, 26, 28, 30 and 60, in both neutral and multiple positive and negative charge states. The results are of use, notably, for direct comparison with observed IR absorption in the interstellar medium. Frequencies fall typically into two ranges, with C−C stretch modes around 1100–1500 cm −1 (6.7–9.1 μm) and fullerene-specific radial motion associated with under-coordinated carbon at pentagonal sites in the range 600–800 cm −1 (12.5–16.7 μm). Notably, negatively charged fullerenes show significantly stronger absorption intensities than neutral species. The results suggest that small cage fullerenes, and notably metallic endofullerenes, may be responsible for many of the unassigned interstellar IR spectral lines. This article is part of the themed issue ‘Fullerenes: past, present and future, celebrating the 30th anniversary of Buckminster Fullerene’.

Funder

European Union's Horizon 2020 research and innovation programme

Publisher

The Royal Society

Subject

General Physics and Astronomy,General Engineering,General Mathematics

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