| Literature DB >> 27501975 |
Jean-Joseph Adjizian1, Alexis Vlandas2, Jeremy Rio3, Jean-Christophe Charlier1, Chris P Ewels4.
Abstract
We calculate the infrared (IR) absorption spectra using DFT B3LYP(6-311G) for a range of small closed-cage fullerenes, Cn, 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'.Entities:
Keywords: Fourier transform infrared spectroscopy; density functional theory; fullerene; infrared; interstellar; spectroscopy
Year: 2016 PMID: 27501975 PMCID: PMC4978747 DOI: 10.1098/rsta.2015.0323
Source DB: PubMed Journal: Philos Trans A Math Phys Eng Sci ISSN: 1364-503X Impact factor: 4.226