Rotational Spectra of Small PAHs: Acenaphthene, Acenaphthylene, Azulene, and Fluorene
Author(s) -
Sven Thorwirth,
P. Theulé,
C. A. Gottlieb,
Michael McCarthy,
P. Thaddeus
Publication year - 2007
Publication title -
the astrophysical journal
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.376
H-Index - 489
eISSN - 1538-4357
pISSN - 0004-637X
DOI - 10.1086/518026
Subject(s) - acenaphthene , acenaphthylene , azulene , physics , fluorene , ground state , rotational spectroscopy , spectroscopy , spectral line , atomic physics , photochemistry , nuclear magnetic resonance , chemistry , astronomy , phenanthrene , astrobiology , polymer
Pure rotational spectra of four small polycyclic aromatic hydrocarbons have been observed by Fourier transform microwave spectroscopy of a molecular beam in the frequency range from 7 to 37 GHz. Initial searches for acenaphthene (C12H10), acenaphthylene (C12H8), and fluorene (C13H10) were guided by quantum chemical calculations performed at the B3LYP/cc-pVTZ level of theory. All three molecules exhibit b-type rotational spectra and are calculated to be moderately polar, with dipole moments of 0.3Y0.9 D. Close agreement (to better than 1%) between the calculated equilibrium and experimentally derived ground-state rotational constants is achieved. Selected transitions of acenaphthene and fluorene have also been measured in the 3 mm region by conventional free-space absorption spectroscopy, as have transitions of the previously studied azulene (C10H8). The data presented here facilitate deep radio astronomical searches with large radio telescopes. Subject headinggs: astrochemistry — ISM: molecules — molecular data Online material: machine-readable tables
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