Infrared Spectra of Hexa-peri-hexabenzocoronene Cations:HBC+ and HBC2+
arXiv:1809.08798 · doi:10.3847/1538-4357/836/1/28
Abstract
We present the first infrared (IR) gas phase spectrum of a large and astronomically relevant PAH cation (CH, HBC) and its di-cation (CH, HBC). The spectra are recorded via infrared multi-photon dissociation (IRMPD) spectroscopy of ions stored in a quadrupole ion trap, using the intense infrared radiation of a free electron laser in the 5301800 cm (5.618.9 m) range. HBC shows main intense absorption peaks at 762 (13.12), 1060 (9.43), 1192 (8.39), 1280 (7.81), 1379 (7.25) and 1530 (6.54) cm(m), in good agreement with DFT calculations that after scaling to take the anharmonicities effect into account. HBC has its main absorption peaks at 660 (15.15), 766 (13.05), 1054 (9.49), 1176 (8.50), 1290 (7.75), 1370 (7.30) and 1530 (6.54) cm(m). Given the similarity in the cationic and di-cationic spectra, we have not identified an obvious diagnostic signature to the presence of multiply charged PAHs in space. While experimental issues associated with the IRMPD technique preclude a detailed comparison with interstellar spectra, we do note that the strong bands of HBC and HBC at 6.5, 7.7, 8.4 and 13.1 m coincide with prominent aromatic infrared bands (AIBs). HBC has only trio CH groups and the out-of-plane CH bending mode of both HBC cations is measured at 13.1 m, squarely in the range predicted by theory and previously found in studies of small (substituted) PAHs. This study therefore supports the use of AIBs observed in the 1114 m range as a diagnostic tool for the edge topology of large PAHs in space.
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