1999
DOI: 10.1063/1.480439
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Dynamics of Y+H2CO reactions

Abstract: The reactions of ground state yttrium atoms (Y) with formaldehyde (H2CO) have been studied in crossed molecular beams as a function of collision energy (Ecoll). The potential energy barrier for C–H insertion is found to lie below 12 kcal/mol. It is proposed that the reaction is initiated by C–H insertion, producing HYCHO followed by H atom migration forming H2YCO. Although Y–CO bond fission leading to YH2+CO is dominant, a secondary minor channel also leads to the production of YCO+H2. Formation of YCHO+H is n… Show more

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Cited by 24 publications
(42 citation statements)
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References 17 publications
(19 reference statements)
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“…[12] by Eq. [11]. In principle this should allow the orbital corrections to the rotational constants, and therefore the electronic contribution to the inertial defect, to be obtained; in practice, though, the spin-orbit constants ζ α are not known well enough.…”
Section: Discussionmentioning
confidence: 97%
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“…[12] by Eq. [11]. In principle this should allow the orbital corrections to the rotational constants, and therefore the electronic contribution to the inertial defect, to be obtained; in practice, though, the spin-orbit constants ζ α are not known well enough.…”
Section: Discussionmentioning
confidence: 97%
“…As can be seen from Eq. [11], the ratio ε aa /ε bb in the states of YC 2 should be equal to A/B. It is not possible to separate ε bb from ε cc for the ground state of YC 2 because the absence of K = 1 levels has resulted in their being almost totally correlated in a least squares sense.…”
Section: Discussionmentioning
confidence: 98%
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“…86 These dynamics calculations are needed to turn the ab initio results into quantities that can be compared with experiments. Although interest in these light elementary reactions still continues, with the development of powerful theoretical models, attention is turning to more complex systems of significant practical interest such as in catalysis, [87][88][89] atmospheric chemistry, 90-92 interstellar [93][94][95] and planetary chemistry, 96-100 organometallic chemistry, 101-103 and combustion processes. [104][105][106][107][108] Due to the experimental difficulties in generating two unstable reactants simultaneously, only a very few atom-radical reactions have been conducted so far under single collision conditions.…”
Section: The Crossed Molecular Beam Methodsmentioning
confidence: 99%