Calculated trends of OH infrared stretching vibrations with composition and structure in aluminosilicate molecules
- Creators
- Kubicki, J. D.
- Sykes, Dan
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Rossman, George R.
Abstract
Ab initio, molecular orbital calculations have been performed on a variety of hypothetical aluminosilicate molecules to investigate relationships among composition, structure, and infrared spectra of OH. Vibrational analyses of the full-optimized molecular geometries at the 3–21G** level were performed with Gaussian 92 to determine theoretical infrared spectra. Theoretical infrared OH frequencies, ν(OH), shift 10 to 100 cm^(−1) with ionic substitutions. The inverse correlation of theoretical infrared OH intensities with OH stretching frequencies in these aluminosilicate molecules is similar to that observed for aluminosilicate glasses (Paterson 1982). O-H bond lengths, H-bond distances, and H-bond angles correlate with frequency. The dominant factor affecting ν(OH) is the H-bond distance, if this distance is less than 2 Å. Beyond H-bond distances of 2 Å, structural and compositional effects exert competitive influences on ν(OH).
Additional Information
© 1993 Springer-Verlag. Received June 23, 1993; Revised, accepted August 24, 1993. JDK acknowledges the support of the Schlumberger Corporation, NSF grant EAR91-17946 (to G. A. Blake), and NASA grant NAGW 2320 (to E. M. Stolper). DS acknowledges support from NSF grant EAR89-04375 (to P.J. Wyllie). GRR acknowledges support from NSF grant EAR92-18980. Computational facilities were provided by the Molecular Simulation Center (W.A. Goddard) of the Beckman Institute at Caltech, the Pittsburgh Supercomputing Center, and E. M. Stolper.Additional details
- Eprint ID
- 39678
- DOI
- 10.1007/BF00203113
- Resolver ID
- CaltechAUTHORS:20130731-133328345
- Schlumberger Corporation
- NSF
- EAR91-17946
- NASA
- NAGW 2320
- NSF
- EAR89-04375
- NSF
- EAR92-18980
- Created
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2013-08-01Created from EPrint's datestamp field
- Updated
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2021-11-09Created from EPrint's last_modified field
- Caltech groups
- Division of Geological and Planetary Sciences (GPS)