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

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Authors

  • C. A. Gottlieb
  • M. C. McCarthy
  • M. J. Travers
  • J. U. Grabow
  • P. Thaddeus

External Research Organisations

  • Harvard University
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Details

Original languageEnglish
Pages (from-to)5433-5438
Number of pages6
JournalJournal of Chemical Physics
Volume109
Issue number13
Publication statusPublished - 1998

Abstract

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 2Π 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 2Π3/2 for C10H, C12H, and C14H, and 2Π1/2 for C13H. Only three spectroscopic constants in the standard Hamiltonian for a molecule in a 2Π state were required to reproduce the spectra to a few parts in 107: 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 ≥5×109 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.

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Rotational spectra of the carbon chain free radicals C10H, C12H, C13H, and C14H. / Gottlieb, C. A.; McCarthy, M. C.; Travers, M. J. et al.
In: Journal of Chemical Physics, Vol. 109, No. 13, 1998, p. 5433-5438.

Research output: Contribution to journalArticleResearchpeer review

Gottlieb, CA, McCarthy, MC, Travers, MJ, Grabow, JU & Thaddeus, P 1998, 'Rotational spectra of the carbon chain free radicals C10H, C12H, C13H, and C14H', Journal of Chemical Physics, vol. 109, no. 13, pp. 5433-5438. https://doi.org/10.1063/1.477161
Gottlieb, C. A., McCarthy, M. C., Travers, M. J., Grabow, J. U., & Thaddeus, P. (1998). Rotational spectra of the carbon chain free radicals C10H, C12H, C13H, and C14H. Journal of Chemical Physics, 109(13), 5433-5438. https://doi.org/10.1063/1.477161
Gottlieb CA, McCarthy MC, Travers MJ, Grabow JU, Thaddeus P. Rotational spectra of the carbon chain free radicals C10H, C12H, C13H, and C14H. Journal of Chemical Physics. 1998;109(13):5433-5438. doi: 10.1063/1.477161
Gottlieb, C. A. ; McCarthy, M. C. ; Travers, M. J. et al. / Rotational spectra of the carbon chain free radicals C10H, C12H, C13H, and C14H. In: Journal of Chemical Physics. 1998 ; Vol. 109, No. 13. pp. 5433-5438.
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abstract = "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 2Π 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 2Π3/2 for C10H, C12H, and C14H, and 2Π1/2 for C13H. Only three spectroscopic constants in the standard Hamiltonian for a molecule in a 2Π state were required to reproduce the spectra to a few parts in 107: 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 ≥5×109 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.",
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T1 - Rotational spectra of the carbon chain free radicals C10H, C12H, C13H, and C14H

AU - Gottlieb, C. A.

AU - McCarthy, M. C.

AU - Travers, M. J.

AU - Grabow, J. U.

AU - Thaddeus, P.

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N2 - 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 2Π 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 2Π3/2 for C10H, C12H, and C14H, and 2Π1/2 for C13H. Only three spectroscopic constants in the standard Hamiltonian for a molecule in a 2Π state were required to reproduce the spectra to a few parts in 107: 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 ≥5×109 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.

AB - 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 2Π 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 2Π3/2 for C10H, C12H, and C14H, and 2Π1/2 for C13H. Only three spectroscopic constants in the standard Hamiltonian for a molecule in a 2Π state were required to reproduce the spectra to a few parts in 107: 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 ≥5×109 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.

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