Multiply charged naphthalene and its C10H8 isomers: bonding, spectroscopy and implications in AGN environments

TL;DR

This study explores the structures, spectra, and stability of multiply charged naphthalene and its isomers, revealing their potential presence and spectral signatures in active galactic nuclei environments.

Contribution

It provides an extensive computational analysis of charged naphthalene isomers, including their structures, spectra, and astrophysical implications, especially in AGN environments.

Findings

Open chains dominate low-energy structures of highly charged isomers.

Simulated IR spectra match experimental data, aiding astronomical observations.

Charged species may contribute to AGN emission spectra.

Abstract

Naphthalene (C10H8) is the simplest polycyclic aromatic hydrocarbon (PAH) and an important component in a series of astrochemical reactions involving hydrocarbons. Its molecular charge state affects the stability of its isomeric structures, which is specially relevant in ionised astrophysical environments. We thus perform an extensive computational search for low-energy molecular structures of neutral, singly, and multiply charged naphthalene and its isomers with charge states +q = 0-4 and investigate their geometric properties and bonding situations. We find that isomerisation reactions should be frequent for higher charged states and that open chains dominate their low-energy structures. We compute both the scaled-harmonic and anharmonic infrared spectra of selected low-energy species and provide the calculated scaling factors for the naphthalene neutral, cation, and dication global minima. All simulated spectra reproduce satisfactorily the experimental data and, thus, are adequate for aiding observations. Moreover, the potential presence of these species in the emission spectra of the circumnuclear regions of active galactic nuclei (AGNs), with high energetic X-ray photon fluxes, is explored using the experimental value of the naphthalene photodissociation cross-section, \sigma_{ph-d}, to determine its half-life, t_{1/2}, at a photon energy of 2.5 keV in a set of relevant sources. Finally, we show that the computed IR bands of the triply and quadruply charged species are able to reproduce some features of the selected AGN sources.