Double ionization of quaterrylene (C40H20) in water-ice at 20 K with Lyα (121.6 nm) radiation

@article{Gudipati2006DoubleIO,
  title={Double ionization of quaterrylene (C40H20) in water-ice at 20 K with Ly$\alpha$ (121.6 nm) radiation},
  author={Murthy S. Gudipati and L. J. Allamandola},
  journal={Journal of Physical Chemistry A},
  year={2006},
  volume={110},
  pages={9020-9024}
}
Polycyclic aromatic hydrocarbon (PAH) molecules undergo facile ionization in cryogenic water-ices resulting in near quantitative conversions of neutral molecules to the corresponding singly charged radical cations. Here we report, for the first time, the production and stabilization of a doubly ionized, closed shell PAH in water-ice. The large PAH quaterrylene (QTR, C40H20) is readily photoionized and stabilized as QTR2+ in a water-ice matrix at 20 K. The kinetic analysis of photolysis shows… 

Figures and Tables from this paper

The highly reactive benzhydryl cation isolated and stabilized in water ice.
TLDR
For the first time, a highly electrophilic and extremely reactive secondary carbenium ion can be isolated in a neutral, nucleophilic environment avoiding superacidic conditions.
Photochemistry of the PAH pyrene in water ice: the case for ion-mediated solid-state astrochemistry
Context. Icy dust grains play an important role in the formation of complex molecules in the interstellar medium (ISH). Laboratory studies have mainly focused on the physical interactions and
Photoinduced Reversible Electron Transfer Between the Benzhydryl Radical and Benzhydryl Cation in Amorphous Water-Ice.
TLDR
Applications of ionization of organic matter trapped in water-ice to icy environments in astrophysics and planetary sciences, including Earth, are discussed.
Lyα-induced charge effects of polycyclic aromatic hydrocarbons embedded in ammonia and ammonia:water ice
Infrared emission features assigned to gas phase polycyclic aromatic hydrocarbons (PAHs) are observed in space along many lines of sight. In regions where interstellar ices are present, these
Growth of larger hydrocarbons in the ionosphere of titan.
TLDR
Despite low steady-state concentrations of the dicationic intermediates, kinetic modeling allows predictions about the larger hydrocarbon species present in the ionosphere of Titan, thereby rationalizing the results from the Cassini–Huygens mission which consideration of monocations only cannot explain.
Survival Depth of Organics in Ices under Low-energy Electron Radiation (?2?keV)
Icy surfaces in our solar system are continually modified and sputtered with electrons, ions, and photons from solar wind, cosmic rays, and local magnetospheres in the cases of Jovian and Saturnian
Excited States and Optical Properties of Hydrogen-Passivated Rectangular Graphenes: A Computational Study
TLDR
This work performs large-scale electron-correlated calculations of optoelectronic properties of rectangular graphene-like polycyclic aromatic hydrocarbon molecules and finds that with the increasing size, they develop a strong diradical open-shell character.
Complementary and Emerging Techniques for Astrophysical Ices Processed in the Laboratory
Inter- and circumstellar ices comprise different molecules accreted on cold dust particles. These icy dust grains provide a molecule reservoir where particles can interact and react. As the grain
Chemistry in Water Ices: From Fundamentals to Planetary Applications
Laboratory studies pertinent to the chemistry of ices with and without additional ingredients such as organics is critical to our understanding of how solar system icy bodies from comets and Kuiper
Surface Science Investigations of Icy Mantle Growth on Interstellar Dust Grains in Cooling Environments
Experimental measurements on the thermal and nonthermal behavior of water and other simple molecules, including organic compounds such as methanol and benzene, on model interstellar dust grain and
...
1
2
...

References

Ices on the Satellites of Jupiter, Saturn, and Uranus
Three satellites of Jupiter, seven satellites of Saturn, and five satellites of Uranus show spectroscopic evidence of H 2 O ice on their surfaces, although other details of their surfaces are highly