15min:
HIGH RESOLUTION ROTATIONAL SPECTRA OF THE FCO2 RADICAL IN ITS X2B2 STATE.

PASCAL DRÉAN, ADAM WALTERS, MARCEL BOGEY, Laboratoire de Physique des Lasers, Atomes et Molécules,Centre de Recherches Lasers et Applications, Université des Sciences et Technologies de Lille, Bât P5, 59655 Villeneuve d'Ascq, France; ZDENEK ZELINGER, J. Heyrovský Institute of Physical Chemistry, Academy of Sciences of the Czech Republic, Dolejskova 3, 182 23 Praha 8, Czech Republic; STEFAN SANDER, HELGE WILLNER, Fachbereich 6, Anorganische Chemie, Gerhard-Mercator-Universität GH Duisburg, Lotharstrasse 1, D-47048 Duisburg, Germany; JÜRGEN BREIDUNG, WALTER THIEL, Max-Planck-Institut für Kohlenforschung, D-45470 Mülheim, Germany; HANS BÜRGER, Fachbereich 9, Anorganische Chemie, Bergische Universität GH Wuppertal, Gaussstrasse 20, D-42119 Wuppertal, Germany.

The fluoroformyloxyl FCO2 radical is of atmospheric interest since it may be produced during the stratospheric degradation of HFCs. It is therefore important to characterize this species in order to better understand its atmospheric chemistry. Moreover, FCO2 should be stable enough in the atmosphere so its abundance may allow its detection by spectroscopic methods \footnoteG. A. Argüello, H. Grothe, M. Kronberg, H. Willner and H.-G. Mack J. Phys. Chem. \underline\textbf99, 17525-17531 (1995).. We hence undertook the first high resolution spectroscopic study of FCO2 in the gas phase.

It was possible to study FCO2 in the gas phase by thermolysis of bis-(monofluorocarbonyl peroxide) FC(O)OO(O)CF at a temperature of about 600 K. The rotational spectrum was recorded in the 270 - 345 GHz region, at room temperature at a pressure of 4 mTorr. All the transitions were split into four components due to the spin-spin and spin-rotation interaction.

Ab initio calculations performed at the CCSD(T) level of theory with polarised-valence-triplezeta basis set TZ2Pf with correlation of all electrons were used to predict the spectrum. Due to the symmetry of the 2B state, only transitions with odd Ka were found. All the lines were fitted to an effective Hamiltonian which comprised spin-spin and spin-rotation interactions together with their corresponding centrifugal distortion operators. We used the CALPGM fitting program of Pickett to derive the spectroscopic constants which were all accurately determined up to the quartic centrifugal distortion constants.