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

Research output: Contribution to JournalArticleAcademicpeer-review

Abstract

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 μm 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.

Original languageEnglish
Article numberA130
JournalAstronomy and Astrophysics
Volume628
DOIs
Publication statusPublished - 1 Aug 2019
Externally publishedYes

Funding

This work was supported by The Netherlands Organization for Scientific Research (NWO) and is part of the Dutch Astrochemistry Network (DAN) II (Project No. 648.000.029). We gratefully acknowledge the NWO for the support of the FELIX Laboratory. A.C. is supported by an NWO VENI grant (No. 639.041.543). The theoretical work was performed on the Dutch national e-infrastructure with the support of SURFsara. Furthermore, we would like to thank the FELIX laboratory team for their experimental assistance.

Keywords

  • Astrochemistry
  • Infrared: ISM
  • ISM: molecules
  • Molecular data

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