INFRARED SPECTROSCOPIC CHARACTERIZATION OF TUNGSTEN CARBONYL SPECIES FORMED BY ULTRAVIOLET PHOTOREDUCTION OF SILICA-SUPPORTED W(VI) IN CARBON-MONOXIDE

Citation
Sd. Kohler et Jg. Ekerdt, INFRARED SPECTROSCOPIC CHARACTERIZATION OF TUNGSTEN CARBONYL SPECIES FORMED BY ULTRAVIOLET PHOTOREDUCTION OF SILICA-SUPPORTED W(VI) IN CARBON-MONOXIDE, Journal of physical chemistry, 98(4), 1994, pp. 1276-1281
Citations number
21
Categorie Soggetti
Chemistry Physical
ISSN journal
00223654
Volume
98
Issue
4
Year of publication
1994
Pages
1276 - 1281
Database
ISI
SICI code
0022-3654(1994)98:4<1276:ISCOTC>2.0.ZU;2-G
Abstract
The tungsten carbonyl species that form during ultraviolet photoreduct ion of W6+/SiO2 in CO were analyzed by Fourier transform infrared spec troscopy (FTIR). Two carbonyl species were identified, mer-W(CO)(3) an d cis-W(CO)(2), by the number and intensities of the respective IR pea ks and through isotopic substitution. The C-2v symmetry of mer-W(CO)(3 ) was associated with three IR bands: a very weak (A(1))(1) symmetric trans mode at 2145 cm(-1), a strong B-2 symmetric mode at 2112 cm(-1), and a strong (A(1))(2) antisymmetric mode at 2179 cm(-1) mer-W(CO)(3) was stable at 298 K in 25 Torr of CO. Isothermal evacuation of the me r-W(CO)(3) species resulted in the loss of a single CO ligand, forming cis-W(CO)(2). The W(CO)(2) species formed during both isothermal evac uation of the mer-W(CO)(3) species and during the initial photoreducti on process. cis-W(CO)(2) was identified by its IR spectrum consisting of a strong symmetric mode at 2112 cm(-1) and a strong antisymmetric m ode at 2040 cm(-1).