15min:
MICROWAVE SPECTRUM AND STRUCTURE OF A POLAR DIMER OF N2O.

NICHOLAS R. WALKER, School of Chemistry, University of Bristol, Bristol, BS8 1TS, U.K.; ANDREA J. MINEI, STEWART E. NOVICK, Department of Chemistry, Wesleyan University, Middletown, Connecticut 06459, U.S.A.; AND ANTHONY C. LEGON, School of Chemistry, University of Bristol, Bristol, BS8 1TS, U.K..

Cavity Fourier-Transform microwave spectroscopy has been used to characterise a gas phase, polar dimer of N2O. The polar (N2O)2 unit is generated by co-expansion of a gas sample containing a small percentage of N2O in a helium backing gas. Transitions in the pure rotational spectra of (15N2O)2, (14N15NO)(15N2O), (14N2O)(15N2O) and (14N2O)2 are reported. The measured transitions of (15N2O)2 and (14N15NO)(15N2O) are assigned and fitted to Hamiltonians allowing rotational, centrifugal distortion and 14N nuclear quadrupole coupling constants to be determined. Hyperfine structure is assigned for a single J_K-1'K+1'' rightarrowJ_K-1''K+1'''' transition of both isotopomers of (14N2O)(15N2O). Nuclear quadrupole coupling constants, chibb, are reported for all four 14N nuclei. The measured chibb are in excellent agreement with those structures predicted from the measured rotational constants. The geometry of the molecule is slipped-parallel. The separation between the central nitrogen nuclei of the monomers in the rm^(1) structure is 3.570(12)Å with the two N2O monomers respectively oriented 54.69(68)\circ and 49.85(64)\circ to the a-inertial axis. Simulation of hyperfine structure in the spectrum of the (14N2O)2 isotopomer yields good qualitative agreement with experiment.