ABSTRACT
We present the low temperature gas-phase vibrational spectrum of ionised 1-cyanonaphthalene (1-CNN+) in the mid-infrared region. Experimentally, 1-CNN+ ions are cooled below 10 K in a cryogenic ion trapping apparatus, tagged with He atoms and probed with tuneable radiation. Quantum-chemical calculations are carried out at a density functional theory level. The spectrum is dominated by the CN-stretch at 4.516 µm, with weaker CH modes near 3.2 µm.
ABSTRACT
We present the first experimental vibrational spectra of gaseous oxidized derivatives of C60 in protonated and radical cation forms, obtained through infrared multiple-photon dissociation spectroscopy using the FELIX free-electron laser. Neutral C60O has two nearly iso-energetic isomers: the epoxide isomer in which the O atom bridges a CC bond that connects two six-membered rings and the annulene isomer in which the O atom inserts into a CC bond connecting a five- and a six-membered ring. To determine the isomer formed for C60O+ in our experimentâa question that cannot be confidently answered on the basis of the DFT-computed stabilities aloneâwe compare our experimental IR spectra to vibrational spectra predicted by DFT calculations. We conclude that the annulene-like isomer is formed in our experiment. For C60OH+, a strong OH stretch vibration observed in the 3 µm range of the spectrum immediately reveals its structure as C60 with a hydroxyl group attached, which is further confirmed by the spectrum in the 400-1600 cm-1 range. We compare the experimental spectra of C60O+ and C60OH+ to the astronomical IR emission spectrum of a fullerene-rich planetary nebula and discuss their astrophysical relevance.
