Published May 1, 2021 | Version v1
Journal article

Competitive Dehydrogenation and Backbone Fragmentation of Superhydrogenated PAHs: A Laboratory Study

  • 1. Fysikum, Stockholms Universitet, Stockholm (Sweden)
  • 2. CNR-Istituto di Struttura della Materia, Area della Ricerca di Roma 1, Rome (Italy)
  • 3. School of Chemistry, University of East Anglia, Norwich (United Kingdom)
  • 4. Laboratoire de Chimie Physique Moléculaire, École Polytechnique Fédérale de Lausanne, Lausanne (Switzerland)
  • 5. Elettra Sincrotrone Trieste, Trieste (Italy)

Description

Superhydrogenated polycyclic aromatic hydrocarbons (PAHs) have been suggested to catalyze the formation of H2 in certain regions of space, but it remains unclear under which circumstances this mechanism is viable given the reduced carbon backbone stability of superhydrogenated PAHs. We report a laboratory study on the stability of the smallest pericondensed PAH, pyrene (C16H10+N, with N = 4, 6, and 16 additional H atoms), against photodestruction by single vacuum ultraviolet photons using the photoelectron–photoion coincidence technique. For N = 4, we observe a protective effect of hydrogenation against the loss of native hydrogens, in the form of an increase in the appearance energies of the C 16 H 9 + and C16H8 + daughter ions compared to those reported for pristine pyrene (C16H10). No such effect is seen for N = 6 or 16, where the weakening effect of replacing aromatic bonds with aliphatic ones outweighs the buffering effect of the additional hydrogen atoms. The onset of fragmentation occurs at similar internal energies for N = 4 and 6, but is significantly lower for N = 16. In all three cases, H-loss and CmHn-loss (m ≥ 1, carbon backbone fragmentation) channels open at approximately the same energy. The branching fractions of the primary channels favor H-loss for N = 4, CmHn-loss for N = 16, and are roughly equal for the intermediate N = 6. We conclude that superhydrogenated pyrene is probably too small to support catalytic H2-formation, while trends in the current and previously reported data suggest that larger PAHs may serve as catalysts up to a certain level of hydrogenation.

Availability note (English)

Available from http://dx.doi.org/10.3847/1538-4357/abf354

Additional details

Identifiers

Publishing Information

Journal Title
Astrophysical Journal
Journal Volume
913
Journal Issue
1
Journal Page Range
[10 p.]
ISSN
0004-637X
CODEN
ASJOAB

INIS

Country of Publication
United Kingdom
Country of Input or Organization
International Atomic Energy Agency (IAEA)
INIS RN
53073389
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Descriptors DEI
CARBON; DEHYDROGENATION; HYDROGEN; HYDROGENATION; PYRENE; SPACE; ULTRAVIOLET RADIATION
Descriptors DEC
AROMATICS; CHEMICAL REACTIONS; ELECTROMAGNETIC RADIATION; ELEMENTS; HYDROCARBONS; NONMETALS; ORGANIC COMPOUNDS; POLYCYCLIC AROMATIC HYDROCARBONS; RADIATIONS