INFRARED-SPECTROSCOPY AND AB-INITIO POTENTIAL-ENERGY SURFACE FOR NE-C2H2 AND NE-C2HD COMPLEXES

Citation
Rj. Bemish et al., INFRARED-SPECTROSCOPY AND AB-INITIO POTENTIAL-ENERGY SURFACE FOR NE-C2H2 AND NE-C2HD COMPLEXES, The Journal of chemical physics, 109(20), 1998, pp. 8968-8979
Citations number
68
Categorie Soggetti
Physics, Atomic, Molecular & Chemical
ISSN journal
00219606
Volume
109
Issue
20
Year of publication
1998
Pages
8968 - 8979
Database
ISI
SICI code
0021-9606(1998)109:20<8968:IAAPSF>2.0.ZU;2-M
Abstract
The rotationally resolved spectra of Ne-C2H2 and Ne-C2HD were measured in the region of the asymmetric C-H stretch (nu(3)) band of the acety lene monomer. The transitions in the Ne-C2H2 spectrum are substantiall y broadened by vibrational predissociation, while those of Ne-C2HD are quite narrow. This difference is attributed to the fact that in the f ormer dissociation proceeds through a '''doorway'' state, related to a Fermi resonance involving the bending vibrations of C2H2. In C2HD thi s Fermi resonance is absent. The potential energy surface (PES) for th e Ne-acetylene complex has been computed using symmetry-adapted pertur bation theory. This PES has been fit to an analytic form and applied i n calculations of the rovibrational energy levels of Ne-C2H2 and Ne-C2 HD. From these levels and calculated transition intensities we generat ed the near-infrared spectra of these complexes in the region of the n u(3) band. These complexes may be considered as nearly free internal r otors. For Ne-C2H2 the results obtained from the ground state PES gave semiquantitative agreement with. the measured spectrum. For Ne-C2HD w e could assign all of the (much sharper) lines in the experimental spe ctrum and obtain the nu(3) excited state interaction potential from a fit of the calculated spectrum to the experimental one. The ground sta te ab initio potential was not altered in this fit; the excellent agre ement between the calculated and measured infrared spectrum for Ne-C2H D demonstrates that our Ne-acetylene potential is quite accurate. (C) 1998 American Institute of Physics, [S0021-9606(98)01644-4].