Millimeter and submillimeter wave spectroscopic investigations into the rotation-tunneling spectrum of gGg' ethylene glycol, HOCH2CH2OH

被引:39
作者
Müller, HSP
Christen, D
机构
[1] Univ Cologne, Inst Phys 1, D-50937 Cologne, Germany
[2] Univ Tubingen, Inst Phys & Theoret Chem, D-72076 Tubingen, Germany
关键词
ethylene glycol; conformer; rotational spectroscopy; tunneling; Coriolis interaction; millimeter wave spectroscopy; submillimeter wave spectroscopy;
D O I
10.1016/j.jms.2004.04.009
中图分类号
O64 [物理化学(理论化学)、化学物理学]; O56 [分子物理学、原子物理学];
学科分类号
070203 ; 070304 ; 081704 ; 1406 ;
摘要
The rotation-tunneling spectrum of the second most stable gGg' conformer of ethylene glycol (1,2-ethanediol) in its ground vibrational state has been studied in selected regions between 77 and 579 GHz. Compared to the study of the more stable aGg' conformer, a much larger frequency range was studied, resulting in a much extended frequency list covering similar quantum numbers, J less than or equal to 55 and K-a less than or equal to 19. While the input data were reproduced within experimental uncertainties up to moderately high values of J and K, larger residuals remain at higher quantum numbers. The severe mixing of the states caused by the Coriolis interaction between the two tunneling substates is suggested to provide a considerable part of the explanation. In addition, a Coriolis interaction of the gGg' ground vibrational state with an excited state of the aGg' conformer may also contribute. Relative intensities of closely spaced lines have been investigated to determine the signs of the Coriolis constants between the two tunneling substates relative to the dipole moment components and to estimate the magnitudes of the dipole moment components and the energy difference between the gGg' and the aGg' conformers. Results of ab initio calculations on the total dipole moment and the vibrational spectrum were needed for these estimates. The current analysis is limited to transitions with quantum numbers J less than or equal to 40 and K-a less than or equal to 6 plus those having J less than or equal to 22 and K-a less than or equal to 17 which could be reproduced within experimental uncertainties. The results are aimed at aiding radioastronomers to search for gGg' ethylene glycol in comets and in interstellar space. (C) 2004 Elsevier Inc. All rights reserved.
引用
收藏
页码:298 / 307
页数:10
相关论文
共 17 条
[1]   The millimeter wave spectrum of aGg′ ethylene glycol:: The quest for higher precision [J].
Christen, D ;
Müller, HSP .
PHYSICAL CHEMISTRY CHEMICAL PHYSICS, 2003, 5 (17) :3600-3605
[2]   The rotational-torsional spectrum of the g′Gg conformer of ethylene glycol:: Elucidation of an unusual tunneling path [J].
Christen, D ;
Coudert, LH ;
Larsson, JA ;
Cremer, D .
JOURNAL OF MOLECULAR SPECTROSCOPY, 2001, 205 (02) :185-196
[3]   THE ROTATIONAL CONCERTED TORSIONAL SPECTRUM OF THE G'GA CONFORMER OF ETHYLENE-GLYCOL [J].
CHRISTEN, D ;
COUDERT, LH ;
SUENRAM, RD ;
LOVAS, FJ .
JOURNAL OF MOLECULAR SPECTROSCOPY, 1995, 172 (01) :57-77
[4]   Ethylene glycol in comet C/1995 O1 (Hale-Bopp) [J].
Crovisier, J ;
Bockelée-Morvan, D ;
Biver, N ;
Colom, P ;
Despois, D ;
Lis, DC .
ASTRONOMY & ASTROPHYSICS, 2004, 418 (03) :L35-L38
[5]   Interstellar antifreeze: Ethylene glycol [J].
Hollis, JM ;
Lovas, FJ ;
Jewell, PR ;
Coudert, LH .
ASTROPHYSICAL JOURNAL, 2002, 571 (01) :L59-L62
[6]  
Larsson J. C., UNPUB
[7]   MICROWAVE-SPECTRUM OF ETHYLENE-GLYCOL [J].
MARSTOKK, KM ;
MOLLENDAL, H .
JOURNAL OF MOLECULAR STRUCTURE, 1974, 22 (02) :301-303
[8]  
MASALLA M, 1997, B SOC CHIM FR, V134, P439
[10]  
PAVELEV DG, UNPUB