SPECTROSCOPY AND DYNAMICS OF RARE GAS-SPHERICAL TOP COMPLEXES .2. THEINFRARED-SPECTRUM OF THE NU(3) BAND OF NE-SIH4 (J=1[-0 AND J=0[-1 TRANSITIONS)

Citation
Md. Brookes et al., SPECTROSCOPY AND DYNAMICS OF RARE GAS-SPHERICAL TOP COMPLEXES .2. THEINFRARED-SPECTRUM OF THE NU(3) BAND OF NE-SIH4 (J=1[-0 AND J=0[-1 TRANSITIONS), The Journal of chemical physics, 104(14), 1996, pp. 5391-5405
Citations number
46
Categorie Soggetti
Physics, Atomic, Molecular & Chemical
ISSN journal
00219606
Volume
104
Issue
14
Year of publication
1996
Pages
5391 - 5405
Database
ISI
SICI code
0021-9606(1996)104:14<5391:SADORG>2.0.ZU;2-J
Abstract
The infrared spectrum of the rare gas-spherical top complex Ne-SiH4 ha s been recorded in a supersonic jet in the region of the SiH4 nu(3) tr iply degenerate stretching vibration at similar to 2189 cm(-1). In con trast to the previously measured Ar-SiH4 spectrum which showed almost equal rotational spacings within each band (corresponding to transitio ns between different internal rotor states of SiH4 within the complex) , the Ne-SiH4 spectrum is complex with no obvious regular band structu re. However, by analogy with the Ar-SiH4 spectrum, four bands of the N e-SiH4 have been assigned and analyzed in terms of Hamiltonians incorp orating Coriolis interaction between the angular momentum of the SiH4 monomer unit and the overall end over end rotation of the complex. The se bands correlate with the SiH4 R(0) (K=0<--0, K=1<--0) and P(1) (K=0 <--0, K=0<--1) transitions. Derived rotational constants demonstrate t hat the neon-silane separation (similar to 4.13 Angstrom in the ground vibrational state) is larger than expected by analogy with Ar-SiH4, i ndicative of nearly free internal rotation by the silane monomer unit in Ne-SiH4. The smaller anisotropy of Ne-SiH4 compared with Ar-SiH4 re sults in a new angular momentum coupling scheme. Transitions arising f rom Ne-22-SiH4 correlating to SiH4 R(0) have also been observed and fi tted; the higher than anticipated intensities demonstrate a novel isot ope enrichment effect in the supersonic jet which is discussed. (C) 19 96 American Institute of Physics.