A tentative identification is proposed of the state of CH\*+ which has been detected in energy loss experiments with a lifetime of at least 3 ks. An empirical modification of a calculated potential energy curve is made which yields a well about I eV deep in the repulsive curve of the ground electron
The vinyloxonium cation (CH2CHOH2+)
β Scribed by Ross H. Nobes; Leo Radom
- Book ID
- 103022790
- Publisher
- Elsevier Science
- Year
- 1983
- Tongue
- English
- Weight
- 385 KB
- Volume
- 99
- Category
- Article
- ISSN
- 0009-2614
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β¦ Synopsis
Ab initio molecular orbital calculations with 1.1r~e basis sets and incorporating correlation nre used to cxarninc the structures and relative energies of the vinylownium (CH2CHOH:) and I-hpdro.\_vethyl (CH3CHOll+) cations. The best structure of the vinylo\onium ion hds the OH2 plane perpendicular to the CC0 pldnc. The energy difference between the vinyloxonium and I-hydroxyethyl cations is predicted to be 92 kJ mol-*, substantially grcdtcr than a recent experimental estimate of 41 * 12 kJ nlol-l . 1_ Intrcduction Three C,H,O+ species are well characterized as being distinct, stable isomers in the gas phase [I ] _ These are the I-hydroxyethyl cation (l), the methoxymethyl cation (2) and 0-protonated oximne (3)_ In an earlier theoretical study [ 11, we proposed that the vinyloxonium cation (4) is also likely to be an observable CZH50+ isomer because of its low relative energy and high barriers to intramolecular rearrange-ment_ In fact, Burgers, Terlouw and Holmes (BTH)
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