SIMULATED INFRARED-EMISSION SPECTRA OF HIGHLY EXCITED POLYATOMIC-MOLECULES - A DETAILED MODEL OF THE PAH-UIR HYPOTHESIS

Citation
Dj. Cook et Rj. Saykally, SIMULATED INFRARED-EMISSION SPECTRA OF HIGHLY EXCITED POLYATOMIC-MOLECULES - A DETAILED MODEL OF THE PAH-UIR HYPOTHESIS, The Astrophysical journal, 493(2), 1998, pp. 793-802
Citations number
36
Categorie Soggetti
Astronomy & Astrophysics
Journal title
ISSN journal
0004637X
Volume
493
Issue
2
Year of publication
1998
Part
1
Pages
793 - 802
Database
ISI
SICI code
0004-637X(1998)493:2<793:SISOHE>2.0.ZU;2-P
Abstract
A detailed description of the polycyclic aromatic hydrocarbon (PAH)/un identified infrared band (UIR) mechanism is presented in which experim ental spectral bandshape functions are used to simulate IR emission sp ectra for individual molecules. These spectra are additively superimpo sed to produce a conglomerate spectrum representative of a family of P AH molecules. Ab initio vibrational frequencies and intensities for ni ne PAHs (neutral and cationic) as large as ovalene are used in conjunc tion with measured bandshape and temperature-dependent redshift data t o simulate the UIR bands. The calculated spectra of cations provide a closer match to the UIRs than do those of the neutrals. However, the P AH cations used in the simulations fail to reproduce the details of th e UIR emission spectra. The discrepancies are potentially alleviated i f both larger PAHs and a greater number of PAHs were included in the s imulation.