On-line database of the spectral properties of polycyclic aromatic hydrocarbons
By Giuliano Malloci, Christine Joblin, Giacomo Mulas. 2007
158 citations recorded by the source corpus.
Abstract We present an on-line database of computed molecular properties for a large sample of polycyclic aromatic hydrocarbons in four charge states: −1, 0, +1, and +2. At present our database includes 40 molecules ranging in size from naphthalene and azulene (C 10 H 8 ) up to circumovalene (C 66 H 20 ). We performed our calculations in the framework of the density functional theory (DFT) and the time-dependent DFT to obtain the most relevant molecular parameters needed for astrophysical applications. For each molecule in the sample, our database presents in a uniform way the energetic, rotational, vibrational, and electronic properties. It is freely accessible on the web at http://astrochemistry.ca.astro.it/database/ and http://www.cesr.fr/~joblin/database/ .
Subfields: Astronomy and Astrophysics, Atomic and Molecular Physics, and Optics, Spectroscopy
View Paper: https://www.semanticscholar.org/paper/2a61b249e835a97ccdfd91fe92e18d6447561ad1
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In Astronomy and Astrophysics
- E. Peeters
- L. Allamandola
- C. Bauschlicher
- N. Flagey
- N. Ysard
- F. Boulanger
- Jacques Le Bourlot
- A. Jones
In Atomic and Molecular Physics, and Optics
In Spectroscopy
Citations in the corpus
- The global dust SED: tracing the nature and evolution of dust with DustEM (2010, background): “Recently, Draine & Li (2007) (hereafter DL07) added the constraints provided by the extensive theoretical database of Malloci et al. (2007) to define a new set of band parameters, both for neutral and cationic PAHs.”
- THE NASA AMES POLYCYCLIC AROMATIC HYDROCARBON INFRARED SPECTROSCOPIC DATABASE: THE COMPUTED SPECTRA (2010, unknown): “This database parallels that described by Malloci et al. (2007), which contains a collection of theoretical spectra and molecular information of 40 PAHs in four different charge states.”
- THE INFRARED SPECTRA OF VERY LARGE IRREGULAR POLYCYCLIC AROMATIC HYDROCARBONS (PAHs): OBSERVATIONAL PROBES OF ASTRONOMICAL PAH GEOMETRY, SIZE, AND CHARGE (2009, background): “…containing about 50 or fewer carbon atoms because large PAHs are not readily available for experimental study and computational techniques for such large systems were not practical (Langhoff 1996; Bauschlicher & Langhoff 1997; Langhoff et al. 1998; Malloci et al. 2007; Pathak & Rastogi 2008).”