15min:
THE RADIO SPECTRUM OF THE PHENYL RADICAL.

R. J. MCMAHON, Department of Chemistry, University of Wisconsin, Madison, WI 54601; M. C. MCCARTHY, J. DUDEK, Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, and Division of Engineering and Applied Sciences, Harvard University, Cambridge, MA 02138; J. F. STANTON, Institute for Theoretical Chemistry, Department of Chemistry and Biochemistry, The University of Texas at Austin, Austin, TX 78712; C. A. GOTTLIEB AND P. THADDEUS, Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, and Division of Engineering and Applied Sciences, Harvard University, Cambridge, MA 02138.

The phenyl radical, C6H5, derived from benzene by removal of one hydrogen, was detected at centimeter wavelengths in a pulsed supersonic molecular beam with a Fourier transform microwave spectrometer, and was subsequently observed in a low-pressure dc glow discharge with a free-space millimeter-wave spectrometer. Each rotational transition in the centimeter-wave band consists of many lines closely-spaced in frequency owing to the fine and hyperfine interactions from the unpaired electron and the five hydrogen atoms; owing to the collapse of this structure in the millimeter-wave band, the rotational spectrum greatly simplifies, allowing the most intense transitions in this region to be calculated to high accuracy. In all, 14~rotational transitions between 9~and 40~GHz and 62~transitions between 150 and 350~GHz have been measured for the normal isotopic species, and a comparable number have been measured for fully deuterated C6D5. Three rotational, three centrifugal distortion constants, and one spin-rotation constant reproduce the spectrum of both species at millimeter wavelengths to better than a few parts in 106. The spectroscopic constants are in excellent agreement with recent CCSD(T)/cc-pVTZ calculations, confirming that phenyl is a fairly rigid planar molecule with a small inertial defect comparable to that derived for benzene. Phenyl is an excellent candidate for astronomical detection because it is a fundamental reactive hydrocarbon species that is calculated to possess a dipole moment of 0.9~D.