Competitive Dehydrogenation and Backbone Fragmentation of Superhydrogenated PAHs: A Laboratory Study
Creators
- 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 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/abf354Additional 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