Recurrent Fluorescence of Polycyclic Aromatic Hydrocarbon Isomers: A Comparative Study

Time-dependent unimolecular dissociation rates of the C<sub>12</sub>H<sub>8</sub> isomers acenaphthylene (ACY) and biphenylene (BPY) cations were measured using a cryogenic electrostatic ion beam storage ring. The neutral, cyano-functionalized tracers of ACY, but not of BPY, have been identified in the interstellar molecular cloud TMC-1 by radioastronomy. For both polycyclic aromatic hydrocarbons (PAHs), dissociation is rapidly quenched by recurrent fluorescence (RF). Master equation simulations including RF rate coefficients based on <i>ab initio</i> molecular dynamics calculations reproduce the measured dissociation rates. Only marginal differences in the survival probabilities of ACY and BPY in TMC-1 are indicated by these results, with both cations being stable for vibrational energies up to about 7.6 eV, which is 3 eV above the dissociation threshold energy.

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Journal
ACS Earth and Space Chemistry
Published
2025-11-25
DOI
https://doi.org/10.1021/acsearthspacechem.5c00283
Primary Topic
Astrophysics and Star Formation Studies
Type
article
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article

Recurrent Fluorescence of Polycyclic Aromatic Hydrocarbon Isomers: A Comparative Study

Henning T. Schmidt, Paul Martini, H. Cederquist, Arun Subramani et al.
ACS Earth and Space Chemistry
Astrophysics and Star Formation Studies
article

Recurrent Fluorescence of Polycyclic Aromatic Hydrocarbon Isomers: A Comparative Study

Henning T. Schmidt, Paul Martini, H. Cederquist, Arun Subramani, James N. Bull, Henning Zettergren, Mark H. Stockett
article en

Abstract

Time-dependent unimolecular dissociation rates of the C<sub>12</sub>H<sub>8</sub> isomers acenaphthylene (ACY) and biphenylene (BPY) cations were measured using a cryogenic electrostatic ion beam storage ring. The neutral, cyano-functionalized tracers of ACY, but not of BPY, have been identified in the interstellar molecular cloud TMC-1 by radioastronomy. For both polycyclic aromatic hydrocarbons (PAHs), dissociation is rapidly quenched by recurrent fluorescence (RF). Master equation simulations including RF rate coefficients based on <i>ab initio</i> molecular dynamics calculations reproduce the measured dissociation rates. Only marginal differences in the survival probabilities of ACY and BPY in TMC-1 are indicated by these results, with both cations being stable for vibrational energies up to about 7.6 eV, which is 3 eV above the dissociation threshold energy.

ACS Earth and Space ChemistryVol. 9(12)
University of East Anglia (GB), Stockholm University (SE)
Openalex Percentile: Top 75%
Astrophysics and Star Formation Studies
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