Structures and G3X energies of C3H3N+ intermediates
Article first published online: 19 JUL 2006
DOI: 10.1002/qua.21146
Copyright © 2006 Wiley Periodicals, Inc.
Issue
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International Journal of Quantum Chemistry
Special Issue: Proceedings of the International Symposium on Theory and Computations in Molecular and Materials Sciences, Biology, and Pharmacology
Volume 106, Issue 15, pages 3043–3047, 2006
Additional Information
How to Cite
Elkner, K., Binning, R. C. and Bacelo, D. E. (2006), Structures and G3X energies of C3H3N+ intermediates. Int. J. Quantum Chem., 106: 3043–3047. doi: 10.1002/qua.21146
Publication History
- Issue published online: 26 SEP 2006
- Article first published online: 19 JUL 2006
- Manuscript Accepted: 22 MAR 2006
- Manuscript Received: 26 FEB 2006
- Abstract
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- Cited By
Keywords:
- ab initio;
- potential energy surface;
- cyanoethenyl cation;
- G3X theory;
- interstellar chemistry
Abstract
Geometries and energies of 15 stable C3H3N+ structures, potential intermediates in ion–molecule reactions that occur on the C3H3N+ potential energy surface (PES), have been calculated with G3X theory. Accurate energy ordering of the intermediates is needed to understand the initial stage of the reactions. The reactions of N(2D) with cyclopropenyl cation and of HCN and HNC with acetylene cation radical are of interest because they may lead to the formation of cyanoacetylene or some of its isomers in dense interstellar dust clouds. The energetics of the initial phases of these reactions are discussed in light of the calculated energies of reactants and intermediates. The variety of high-energy intermediates optimized makes it likely that the reactions discussed involve long-lived complexes and multiple rearrangements. © 2006 Wiley Periodicals, Inc. Int J Quantum Chem, 2006

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