Rotational spectra of the carbon chain free radicals C10H, C12H, C13H, and C14H

被引:41
作者
Gottlieb, CA [1 ]
McCarthy, MC
Travers, MJ
Grabow, JU
Thaddeus, P
机构
[1] Harvard Univ, Div Engn & Appl Sci, Cambridge, MA 02138 USA
[2] Harvard Smithsonian Ctr Astrophys, Cambridge, MA 02138 USA
关键词
D O I
10.1063/1.477161
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 four carbon chain radicals C10H, C12H, C13H, and C14H have been observed in a pulsed supersonic molecular beam with a Fourier transform microwave spectrometer. The radicals were produced in a discharge through a dilute diacetylene/neon mixture in the throat of a supersonic nozzle. All are linear with (2)Pi electronic ground states, and all except C14H have resolved lambda-type doubling. For each species at least ten rotational transitions, between 6 and 16 GHz, were measured in the lowest spin component, which is (2)Pi(3/2) for C10H, C12H, and C14H, and (2)Pi(1/2) for C13H Only three spectroscopic constants in the standard Hamiltonian for a molecule in a (2)Pi state were required to reproduce the spectra to a few parts in 10(7): an effective rotational constant, a centrifugal distortion constant, and a lambda-type doubling constant. All of the chains here have abundances in the most intense part of the supersonic molecular beam of greater than or equal to 5 x 10(9) per gas pulse, which suggests that optical transitions of all four may be detectable with present laser techniques. For the carbon chain radicals with an even number of carbon atoms, there is very little change in relative abundance from C6H to C14H. (C) 1998 American Institute of Physics. [S0021-9606(98)00230-X].
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页码:5433 / 5438
页数:6
相关论文
共 27 条
[1]  
BITTNER JD, 1982, 19TH S INT COMB PITT, P211
[2]   EFFECTIVE HAMILTONIAN FOR DIATOMIC-MOLECULES - ABINITIO CALCULATIONS OF PARAMETERS OF HCL+ [J].
BROWN, JM ;
COLBOURN, EA ;
WATSON, JKG ;
WAYNE, FD .
JOURNAL OF MOLECULAR SPECTROSCOPY, 1979, 74 (02) :294-318
[3]  
Cernicharo J, 1996, ASTRON ASTROPHYS, V309, pL27
[4]   THE FORMATION OF CYANOPOLYYNE MOLECULES IN IRC+10216 [J].
CHERCHNEFF, I ;
GLASSGOLD, AE ;
MAMON, GA .
ASTROPHYSICAL JOURNAL, 1993, 410 (01) :188-201
[5]  
CRAWFORD TD, UNPUB
[6]  
DIXON TA, 1977, J CHEM PHYS, V67, P3956, DOI 10.1063/1.435412
[7]   ELECTRONIC ABSORPTION-SPECTRA OF LINEAR CARBON CHAINS IN NEON MATRICES .2. C-2N(-), C-2N, AND C2NH [J].
FREIVOGEL, P ;
FULARA, J ;
JAKOBI, M ;
FORNEY, D ;
MAIER, JP .
JOURNAL OF CHEMICAL PHYSICS, 1995, 103 (01) :54-59
[8]  
Guelin M, 1997, ASTRON ASTROPHYS, V317, pL1
[9]  
Herzberg G, 1950, Molecular spectra molecular structure: Spectra of diatomic molecules, VI
[10]   MICROWAVE AND INFRARED-SPECTRA OF FREE-RADICALS AND MOLECULAR-IONS [J].
HIROTA, E .
CHEMICAL REVIEWS, 1992, 92 (01) :141-173