arXiv Analytics

Sign in

arXiv:1907.09351 [astro-ph.GA]AbstractReferencesReviewsResources

Anharmonicity in the mid-infrared spectra of polycyclic aromatic hydrocarbons: Molecular beam spectroscopy and calculations

A. K. Lemmens, D. B. Rap, J. M. M. Thunnissen, C. J. Mackie, A. Candian, A. G. G. M. Tielens, A. M. Rijs, W. J. Buma

Published 2019-07-22Version 1

Aims. In this work we determine the effects of anharmonicity on the mid-infrared spectra of the linear polycyclic aromatic hydrocarbons (PAHs) naphthalene, anthracene, tetracene and pentacene recorded using the free electron laser FELIX. Methods. Comparison of experimental spectra obtained under supersonic jet conditions with theoretically predicted spectra was used to show if anharmonicity explicitly needs to be taken into account. Results. Anharmonic spectra obtained using second-order vibrational perturbation theory agree on average within 0.5% of the experimental frequencies. Importantly, they confirm the presence of combination bands with appreciable intensity in the 5-6 $\mu$m region. These combination bands contain a significant fraction of the IR absorption, which scales linearly with the size of the PAH. Detection and assignment of the combination bands are a preliminary indication of the accuracy of far-IR modes in our anharmonic theoretical spectra. Detailed analysis of the periphery-sensitive CH out-of-plane band of naphthalene reveals that there is still room for improvement of the VPT2 approach. In addition, the implications of our findings for the analysis of the aromatic infrared bands are discussed.

Comments: 10 pages, 3 figures and Appendix. Accepted in Astronomy and Astrophysics
Related articles: Most relevant | Search more
arXiv:1710.01835 [astro-ph.GA] (Published 2017-10-05)
Cross section alignment of polycyclic aromatic hydrocarbons by anisotropic radiation
arXiv:2011.10114 [astro-ph.GA] (Published 2020-11-19)
The properties of Polycyclic Aromatic Hydrocarbons in galaxies: constraints on PAH sizes, charge and radiation fields
arXiv:2402.07989 [astro-ph.GA] (Published 2024-02-12, updated 2024-09-08)
A new census of dust and polycyclic aromatic hydrocarbons at z=0.7-2 with JWST MIRI