1976
DOI: 10.1139/v76-201
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Structure of radicals produced by γ-radiolysis. Part 5. Radicals derived from some aliphatic alkene molecules

Abstract: Adamantane isolation matrices have been used to determine the structure of radicals produced by room temperature γ-radiolysis of certain selected alkene systems. The molecules studied include linear 1-ene homologues, linear 2-ene homologues, 2-methylpropene (2MPr), 2-methylbutene-1 (2MB1), 3-methylbutene-1 (3MB1), 2-methylbutene-2 (2MB2), 2-methylpentene-1 (2MP1), 2-methylpentene-2 (2MP2), 4-methylpentene-2 (4MP2), 2,3-dimethylbutene-2 (DMB2), 3,3-dimethylbutene-1 (33DMB), and 2,4,4-trimethylpentene-1 (TMPE). … Show more

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Cited by 21 publications
(4 citation statements)
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“…This is reminiscent of the 14.4 G splitting observed for the spectra of neutral allyl radicals obtained from olefins in Freon matrices, , where the small difference of ca. 0.8 G between the α-couplings from unsubstituted exo - and endo -1,3-hydrogens is typically not resolved.…”
Section: Resultsmentioning
confidence: 99%
“…This is reminiscent of the 14.4 G splitting observed for the spectra of neutral allyl radicals obtained from olefins in Freon matrices, , where the small difference of ca. 0.8 G between the α-couplings from unsubstituted exo - and endo -1,3-hydrogens is typically not resolved.…”
Section: Resultsmentioning
confidence: 99%
“…9). This signal consisted of an apparent six-line spectrum with a hyperfine coupling of approximately 1.7 G. The line shape and hyperfine coupling were clearly inconsistent with a signal arising from the dimethylallyl radical 13 (26). However, the four hydrogens of the methylene groups and the aldehydic hydrogen of the radical 12 would be expected to couple to the free radical to produce the observed spectrum.…”
mentioning
confidence: 92%
“…Because of its unique reactivity of taking part in a series of free radical reactions, NO attracts interest among theoretical physicists and chemists, and reaction mechanisms of a variety of free radicals like CH 3 O 2 [2], OBrO [3], CH 3 S [4], C 2 (a 3 Π u ) [5], NCS [6], CH 3 [7,8], H 2 [9], XCO (X=H,F,Cl) [10], and NH(D) [11] with NO have been reported. C 3 H 5 , which is isomeric with allyl and glyceryl, plays an important role in combustion processes, photochemistry and interstellar chemistry [12,13]. C 3 H 5 • has three isomers: allyl, 1-propenyl, and 2-propenyl.…”
Section: Introductionmentioning
confidence: 99%