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Locally Aromatic Polycyclic Hydrocarbons as Potential Carriers of Infrared Emission Features

Petrie, Simon; Stranger, Robert; Duley, Walter

Description

We report B-LYP/6-31G* and B3-LYP/6-31G* density functional theory calculations on a set of polycyclic hydrocarbons, ranging in size from C19H22 to C36H32, combining aromatic (unsaturated) and aliphatic (saturated, sp3-hybridized carbon) ring systems. These locally aromatic polycyclic hydrocarbons (LAPHs), generally exhibiting large deviations from planarity, may be considered as intermediate structures between polycyclic aromatic hydrocarbons (PAHs) and nanodiamonds. Calculated infrared...[Show more]

dc.contributor.authorPetrie, Simon
dc.contributor.authorStranger, Robert
dc.contributor.authorDuley, Walter
dc.date.accessioned2015-12-13T22:36:44Z
dc.date.available2015-12-13T22:36:44Z
dc.identifier.issn0004-637X
dc.identifier.urihttp://hdl.handle.net/1885/76912
dc.description.abstractWe report B-LYP/6-31G* and B3-LYP/6-31G* density functional theory calculations on a set of polycyclic hydrocarbons, ranging in size from C19H22 to C36H32, combining aromatic (unsaturated) and aliphatic (saturated, sp3-hybridized carbon) ring systems. These locally aromatic polycyclic hydrocarbons (LAPHs), generally exhibiting large deviations from planarity, may be considered as intermediate structures between polycyclic aromatic hydrocarbons (PAHs) and nanodiamonds. Calculated infrared vibrational frequencies are found to be similar to those observed experimentally in spectra of hydrogenated amorphous carbon (HAC) and other carbonaceous solids. In the C-H stretching region (∼3.1-3.6 μm) these species are characterized by strong absorption/emission within both the aliphatic and aromatic C-H bands. They also show spectral features associated with tertiary C-H. Similar features are evident in calculated spectra of the corresponding ions, which we have characterized in some cases. Ionization results in the particular enhancement of a spectral feature typically seen at ∼6.4 μm, in the aromatic C-C stretching region. In keeping with previous experimental and theoretical studies on the spectra of neutral and cationic PAHs, we find that the influence of ionization on the relative intensities of C-C and C-H stretching features is much greater than the influence of molecular structure. We suggest that LAPHs may be significant contributors to emission in Type B unidentified infrared emission sources.
dc.publisherIOP Publishing
dc.sourceAstrophysical Journal, The
dc.subjectKeywords: Astrochemistry; Circumstellar matter; Dust, extinction; Infrared: ISM; ISM: molecules; Molecular data
dc.titleLocally Aromatic Polycyclic Hydrocarbons as Potential Carriers of Infrared Emission Features
dc.typeJournal article
local.description.notesImported from ARIES
local.description.refereedYes
local.identifier.citationvolume594
dc.date.issued2003
local.identifier.absfor030701 - Quantum Chemistry
local.identifier.ariespublicationMigratedxPub5722
local.type.statusPublished Version
local.contributor.affiliationPetrie, Simon, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationStranger, Robert, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationDuley, Walter, University of Waterloo
local.bibliographicCitation.startpage869
local.bibliographicCitation.lastpage873
local.identifier.doi10.1086/377119
dc.date.updated2015-12-11T09:33:25Z
local.identifier.scopusID2-s2.0-0242676890
CollectionsANU Research Publications

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