15min:
INFRARED SPECTRA OF C2H4 UNDER JET-COOLED AND PARA-H2 MATRIX CONDITIONS .

YUAN-PERN LEE AND CHUNG-WEI HUANG, Department of Applied Chemistry and Institute of Molecular Science, National Chiao Tung University, Hsinchu 30010, Taiwan and Institute of Atomic and Molecular Sciences, Academia Sinica, Taipei 10617, Taiwan; KEEVIN DIDRICHE AND MICHEL HERMAN, Laboratoire de Chimie quantique et Photophysique, CP160/09, Université libre de Bruxelles, Ave. Roosevelt, 50, B-1050, Brussels, Belgium; MAUD ROTGER, Institut Carnot de Bourgogne, UMR 5209 CNRS-Université de Bourgogne, 9 avenue Alain Savary, B.P. 47870, F-21078 Dijon Cedex, France.

Spectra of C2H4 isolated in para-H2 are compared with those of jet-cooled C2H4 recorded with an FTIR spectrometer. The nu 7, nu 9, and nu 11 bands of jet-cooled C2H4 all exhibit an intensity distribution corresponding to about 10 K for rotation, with no evidence of nuclear spin conversion. Spectra of the nu 11 band of C2H4 isolated in solid para-H2 clearly show a rotational structure similar to that observed for C2H4 in helium droplets. Other bands of C2H4 exhibit only partially resolved rotational structures. Rotational constants B and C for nu 11 of C2H4 in para-H2 are about 50 % those of the gaseous C2H4. The out-of-plane deformation mode nu 7 shows a small (< 1 cm-1) blue matrix shift, whereas other modes are red-shifted by 2.2 to 3.9 cm-1.