HIGH-RESOLUTION FOURIER-TRANSFORM MICROWAVE SPECTROSCOPY OF METHYL- AND DIMETHYLNAPTHALENES

被引:12
|
作者
Schnitzler, Elijah G. [1 ]
Zenchyzen, Brandi L. M. [1 ]
Jaeger, Wolfgang [1 ]
机构
[1] Univ Alberta, Dept Chem, Edmonton, AB T6G 2G2, Canada
来源
ASTROPHYSICAL JOURNAL | 2015年 / 805卷 / 02期
基金
加拿大自然科学与工程研究理事会;
关键词
astrochemistry; ISM: molecules; molecular data; POLYCYCLIC AROMATIC-HYDROCARBONS; MILLIMETER-WAVE SPECTROSCOPY; LARGE-AMPLITUDE MOTIONS; EMISSION; SPECTRUM; PANHS; PAHS;
D O I
10.1088/0004-637X/805/2/141
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
High-resolution pure rotational spectra of four alkylnaphthalenes were measured in the range of 6-15 GHz using a molecular-beam Fourier-transform microwave spectrometer. Both a-and b-type transitions were observed for 1-methylnaphthalene (1-MN), 1,2-dimethylnaphthalene (1,2-DMN), and 1,3-dimethylnaphthalene (1,3-DMN); only a-type transitions were observed for 2-methylnaphthalene (2-MN). Geometry optimization and vibrational analysis calculations at the B3LYP/ 6-311++ G(d, p) level of theory aided in the assignments of the spectra and the characterization of the structures. Differences between the experimental and predicted rotational constants are small, and they can be attributed in part to low-lying out-of-plane vibrations, which distort the alkylnaphthalenes out of their equilibrium geometries. Splittings of rotational lines due to methyl internal rotation were observed in the spectra of 2-MN, 1,2-DMN, and 1,3-DMN, and allowed for the determination of the barriers to methyl internal rotation, which are compared to values from density functional theory calculations. All four species are moderately polar, so they are candidate species for detection by radio astronomy, by targeting the transition frequencies reported here.
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页数:7
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