Lowest bending mode of 13C-substituted C3 and an experimentally derived structure

被引:20
作者
Breier, Alexander A. [1 ]
Buechling, Thomas [1 ]
Schnierer, Rico [2 ]
Lutter, Volker [1 ]
Fuchs, GuidoW. [1 ]
Yamada, Koichi M. T. [3 ]
Mookerjea, Bhaswati [4 ]
Stutzki, Juergen [5 ]
Giesen, Thomas F. [1 ]
机构
[1] Univ Kassel, Inst Phys, Astrophys Lab, D-34132 Kassel, Germany
[2] Univ Rostock, Inst Phys, Phys New Mat, D-18059 Rostock, Germany
[3] AIST, EMTech, Onogawa 16-1, Tsukuba, Ibaraki 3058569, Japan
[4] Tata Inst Fundamental Res, Homi Bhabha Rd, Bombay 400005, Maharashtra, India
[5] Univ Cologne, Phys Inst 1, D-50937 Cologne, Germany
关键词
DIODE-LASER SPECTROSCOPY; CARBON CLUSTERS; BAND; MOLECULES; SPECTRA; LINES; C-12; CCC;
D O I
10.1063/1.4971854
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
The nu(2) lowest bending mode of linear C-3 and of all its C-13-substituted isotopologues was recorded using a terahertz-supersonic jet spectrometer in combination with a laser ablation source. Sixty-five ro-vibrational transitions between 1.8 and 1.9 THz have been assigned to linear (CCC)-C-12-C-12-C-12, (CCC)-C-12-C-12-C-13, (CCC)-C-12-C-13-C-12, (CCC)-C-13-C-13-C-12, (CCC)-C-13-C-12-C-13, and (CCC)-C-13-C-13-C-13. For each isotopologue, molecular parameters were obtained and the C-C-bond length was derived experimentally. All results are in excellent agreement with recent ab initio calculations [B. Schroder and P. Sebald, J. Chem. Phys. 144, 044307 (2016)]. The new measurements explain why the interstellar search for singly substituted (CCC)-C-12-C-12-C-13 has failed so far. A spectral line list with recommended transition frequencies based on global data fits is given to foster future interstellar detections. Published by AIP Publishing.
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页数:10
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