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PAH Products and Processing by Different Energy SourcesIsoviolanthrene (C34H18), a polycyclic aromatic hydrocarbon (PAH) molecule, was studied via matrix isolation in argon and water at 20 K. Infrared spectroscopy was performed in situ where samples were irradiated using ultraviolet light. Experimental spectra were compared to theoretical spectra for vibrational band assignment, determination of the corresponding A-values, and photoproduct identification. Isoviolanthrene was also deposited as a thin film and irradiated with different energy sources: ultraviolet photons (10.2 eV), soft electrons (1.5 keV), protons (1.5 MeV), and He+ particles (1.5 MeV), to understand the effects of different energy sources on a PAH. Anions and cations of soviolanthrene were produced as a result of UV photolysis in an argon matrix. Hydrogenand oxygen-rich aromatic photoproducts were produced by ultraviolet photons when isoviolanthrene was isolated in a water matrix. The irradiated PAH thin films results were dependent on the energy source. Irradiation with ultraviolet photons yielded a broad underlying feature centered at 9.6 μm, while bombardment with soft electrons gave a broad feature centered at 7.7 μm. In the case of proton bombardment, no broad feature was detected, in contrast with He+ bombardment that destroyed most of the isoviolanthrene and produced broad features in the C-Hoop and C–H stretching regions. A comparison of astronomical IR emission observations with our experimental results in the mid-infrared range has revealed a similarity between the observed plateaus and the broad features produced by our experiments.
Document ID
20205004452
Acquisition Source
Ames Research Center
Document Type
Reprint (Version printed in journal)
Authors
G. A. Cruz-Diaz
(Bay Area Environmental Research Institute Petaluma, California, United States)
S. E. Erickson
(University of Minnesota, Duluth Duluth, Minnesota, United States)
E. F. da Silveira
(Pontifical Catholic University of Rio de Janeiro Rio de Janeiro, Brazil)
A. L. F. de Barros
(Federal Center for Technological Education Celso Suckow da Fonseca Rio de Janeiro, Brazil)
C. A. P. da Costa
(Pontifical Catholic University of Rio de Janeiro Rio de Janeiro, Brazil)
R. C. Pereira
(Federal Center for Technological Education Celso Suckow da Fonseca Rio de Janeiro, Brazil)
A. L. Mattioda
(Ames Research Center Mountain View, California, United States)
Date Acquired
July 14, 2020
Publication Date
September 1, 2019
Publication Information
Publication: The Astrophysical Journal
Publisher: IOP Science
Volume: 882
Issue: 1
ISSN: 0004-637X
e-ISSN: 1538-4357
Subject Category
Chemistry And Materials (General)
Funding Number(s)
WBS: 811073.02.52.01.33
Distribution Limits
Public
Copyright
Public Use Permitted.
Technical Review
Single Expert
Keywords
astrochemistry – infrared: ISM – methods: laboratory: molecular – molecular processes – techniques: spectroscopic
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