On the Interaction of Methyl Azide (CH3N3) Ices with Ionizing Radiation: Formation of Methanimine (CH2NH), Hydrogen Cyanide (HCN), and Hydrogen Isocyanide (HNC)
Autor: | Alfredo Quinto-Hernandez, Chris J. Bennett, Ralf I. Kaiser, Y. S. Kim, Alec M. Wodtke |
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Rok vydání: | 2010 |
Předmět: |
Azides
Solar System Spectrophotometry Infrared Astrophysics::High Energy Astrophysical Phenomena Hydrogen isocyanide Hydrogen cyanide Cosmic ray Electron Photochemistry Ionizing radiation chemistry.chemical_compound chemistry Hydrogen Cyanide Radiation Ionizing Molecule Imines Astrophysics::Earth and Planetary Astrophysics Physical and Theoretical Chemistry Cyanates Astrophysics::Galaxy Astrophysics Methyl azide |
Zdroj: | The Journal of Physical Chemistry A |
ISSN: | 1520-5215 1089-5639 |
DOI: | 10.1021/jp103028v |
Popis: | Methyl azide (CH(3)N(3)) might be a potential precursor in the synthesis of prebiotic molecules via nonequilibrium reactions on interstellar ices initiated by energetic galactic cosmic rays (GCR) and photons. Here, we investigate the effects of energetic electrons as formed in the track of cosmic ray particles and 193 nm photons with solid methyl azide at 10 K and the inherent formation of methanimine (CH(2)NH), hydrogen cyanide (HCN), and hydrogen isocyanide (HNC). We present a systematic kinetic study and outline feasible reaction pathways to these molecules. These processes might be also important in solar system analogue ices. |
Databáze: | OpenAIRE |
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