Cationic Methylene-Pyrene Isomers and Isomerization Pathways: Finite Temperature Theoretical Studies

被引:23
作者
Rapacioli, Mathias [1 ,2 ]
Simon, Aude [1 ,2 ]
Marshall, Charlotte C. M. [3 ,4 ]
Cuny, Jerome [1 ,2 ]
Kokkin, Damian [3 ,4 ]
Spiegelman, Fernand [1 ,2 ]
Jobin, Christine [3 ,4 ]
机构
[1] Univ Toulouse UPS, Lab Chim & Phys Quant LCPQ IRSAMC, 118 Route Narbonne, F-31062 Toulouse, France
[2] CNRS, F-31062 Toulouse, France
[3] Univ Toulouse, IRAP, UPS OMP, F-31400 Toulouse, France
[4] CNRS, IRAP, F-31028 Toulouse 4, France
关键词
POLYCYCLIC AROMATIC-HYDROCARBONS; DENSITY-FUNCTIONAL THEORY; TIGHT-BINDING METHOD; INFRARED-SPECTRA; MOLECULAR-DYNAMICS; EXCITATION-ENERGIES; COMPLEX MATERIALS; DFTB PARAMETERS; PERIODIC-TABLE; SPECTROSCOPY;
D O I
10.1021/acs.jpca.5b09494
中图分类号
O64 [物理化学(理论化学)、化学物理学];
学科分类号
070304 ; 081704 ;
摘要
This paper provides spectral characterizations of the two isomers of the 1-ethylenepyrene cation, namely, the 1-pyrenemethylium and a pyrene-like isomer owing a tropylium cycle. Both are possible photodissociation products of the 1-methylpyrene cation and were proposed as potential contributors to the diffuse interstellar bands. In that respect, vibrational and electronic spectra are computed for the optimized structures at the density functional theory (DFT) and time-dependent (TD-)DFT levels. Finite temperature effects on these spectra are estimated from molecular dynamics simulations within the density functional-based tight-binding (DFTB) and TD-DFTB frameworks, these methods being first benchmarked against DFT and TD-DFT calculations. The computed spectra allow discrimination of the two isomers. When the temperature increases, bands are observed to redshift and merge. The isomerization mechanism is investigated with the metadynamics technique, a biased dynamics scheme allowing to probe reaction mechanisms with high energy barriers by investigating the free energy surface at various temperatures. Four pathways with similar barrier heights (3.5-4 eV) are found, showing that the interconversion process would only occur in interstellar clouds under photoactivation. The present study opens the way to simulations on larger methyl- and methylenePAHs of astrophysical interest and their experimental investigation.
引用
收藏
页码:12845 / 12854
页数:10
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