Infrared Spectra of Hexa-peri-hexabenzocoronene Cations:HBC+ and HBC2+ (1809.08798v1)

Abstract: We present the first infrared (IR) gas phase spectrum of a large and astronomically relevant PAH cation (C${42}$H${18}$$^+$, HBC$^+$) and its di-cation (C${42}$H${18}$$^{2+}$, HBC$^{2+}$). The spectra are recorded via infrared multi-photon dissociation (IRMPD) spectroscopy of ions stored in a quadrupole ion trap, using the intense infrared radiation of a free electron laser in the 530$-$1800 cm$^{-1}$ (5.6$-$18.9 $\mu$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$^{-1}$($\mu$m), in good agreement with DFT calculations that after scaling to take the anharmonicities effect into account. HBC$^{2+}$ 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$^{-1}$($\mu$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$^{2+}$ at $\sim$ 6.5, 7.7, 8.4 and 13.1 $\mu$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 $\mu$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 11$-$14 $\mu$m range as a diagnostic tool for the edge topology of large PAHs in space.