Gas-phase spectroscopy of photostable PAH ions from the mid- to far-infrared

Author:

Wiersma Sandra D123ORCID,Candian Alessandra1ORCID,Bakker Joost M2ORCID,Petrignani Annemieke1ORCID

Affiliation:

1. Van ‘t Hoff Institute for Molecular Sciences, University of Amsterdam , PO Box 94157, NL-1090 GD Amsterdam, The Netherlands

2. Radboud University, Institute for Molecules and Materials, FELIX Laboratory , Toernooiveld 7, NL-6525 ED Nijmegen, The Netherlands

3. Institut de Recherche en Astrophysique et Planétologie (IRAP), CNRS, Université de Toulouse (UPS) , F-31028 Toulouse, France

Abstract

ABSTRACT We present gas-phase InfraRed Multiple Photon Dissociation (IRMPD) spectroscopy of cationic phenanthrene, pyrene, and perylene over the 100–1700 cm−1 (6–95 μm) spectral range. This range covers both local vibrational modes involving C–C and C–H bonds in the mid-IR, and large-amplitude skeletal modes in the far-IR. The experiments were done using the 7T Fourier-Transform Ion Cyclotron Resonance (FTICR) mass spectrometer integrated in the Free-Electron Laser for Intra-Cavity Experiments (FELICE), and findings were complemented with Density Functional Theory (DFT) calculated harmonic and anharmonic spectra, matching the experimental spectra well. The experimental configuration that enables this sensitive spectroscopy of the strongly bound, photoresistant Polycyclic Aromatic Hydrocarbons (PAHs) over a wide range can provide such high photon densities that even combination modes with calculated intensities as low as 0.01 km mol−1 near 400 cm−1 (25 μm) can be detected. Experimental frequencies from this work and all currently available IRMPD spectra for PAH cations were compared to theoretical frequencies from the NASA Ames PAH IR Spectroscopic Database to verify predicted trends for far-IR vibrational modes depending on PAH shape and size, and only a relatively small redshift (6–11 cm−1) was found between experiment and theory. The absence of spectral congestion and the drastic reduction in bandwidth with respect to the mid-IR make the far-IR fingerprints viable candidates for theoretical benchmarking, which can aid in the search for individual large PAHs in the interstellar medium.

Funder

NWO

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

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