From planes to bowls: photodissociation of the bisanthenequinone cation
arXiv:1809.09880 · doi:10.1016/j.cplett.2017.12.043
Abstract
We present a combined experimental and theoretical study of the photodissociation of the bisanthenequinone (C28H12O2) cation, Bq+. The experiments show that, upon photolysis, the Bq+ cation does not dehydrogenate, but instead fragments through the sequential loss of the two neutral carbonyl groups, causing the formation of five-membered carbon cycles. Quantum chemical calculations confirm this Bq+ -> [Bq - CO]+ -> [Bq - 2CO]+ sequence as the energetically most favorable reaction pathway. For the first CO loss, a transition state with a barrier of ~3.2 eV is found, substantially lower than the lowest calculated H loss dissociation pathway (~ 4.9 eV). A similar situation applies for the second CO loss channel (~3.8 eV vs. ~4.7 eV), but where the first dissociation step does not strongly alter the planar PAH geometry, the second step transforms the molecule into a bowl-shaped one.
References in corpus (5)
- Formation of buckminsterfullerene (C60) in interstellar space
- Are PAHs precursors of small hydrocarbons in Photo--Dissociation Regions? The Horsehead case
- Laboratory formation of fullerenes from PAHs: Top-down interstellar chemistry
- Laboratory Photo-chemistry of PAHs: Ionization versus Fragmentation
- PAH chemistry at eV internal energies. 2. Ring alteration and dissociation
Cited by in corpus (6)
- Laboratory photo-chemistry of covalently bonded fluorene clusters: observation of an interesting PAH bowl-forming mechanism
- Intermediate-size fullerenes as degradation products of interstellar PAHs
- Synthesizing carbon nanotubes in space
- Fragmentation and isomerization of polycyclic aromatic hydrocarbons in the interstellar medium: coronene as a case study
- Correlation between UV resilience and wavelength of narrow DIBs
- Carbon accretion and desorption by interstellar polycyclic aromatic hydrocarbons