The Journal of Physical Chemistry A · 1999 · 42 citations · 23 references
Natural SciencesChemistryPhysicsChemical KineticsOrganic ChemistryPhysical ChemistryChemical Kinetics ModelingChemical Reaction KineticsChemical ThermodynamicsKinetic ModelingRadical ReactionsReaction MechanismsArrhenius EquationLaser PhotolysisPhotolysisRate ConstantsReaction Rate CoefficientsTemperature Dependence Of Rate CoefficientsTemperature Dependence Of RatesTransient Absorption Spectroscopy
Low-temperature rate coefficients for the reactions C 2 H + C 3 H 4 → products [C 3 H 4 = methylacetylene (propyne) CH 3 CCH and allene (propadiene) CH 2 CCH 2 ] are measured over the temperature range of 155−298 K. Absolute rate constants are determined using laser photolysis and transient infrared absorption spectroscopy. Both reactions are fast, approaching the kinetic limit and have either no temperature dependence or a slight negative temperature dependence. Over the experimental temperature range, the rate constants are fit to the following Arrhenius expressions: k CH 3 CCH = (1.6 ± 0.4) × 10 -10 exp[(71 ± 50)/ T ] cm 3 molecule -1 s -1 and k CH 2 CCH 2 = (1.3 ± 0.6) × 10 -10 exp[(103 ± 136)/ T ] cm 3 molecule -1 s -1 . The corresponding rate constants at 298 K are k CH 3 CCH = (1.9 ± 0.3) × 10 -10 cm 3 molecule -1 s -1 and k CH 2 CCH 2 = (1.7 ± 0.3) × 10 -10 cm 3 molecule -1 s -1 . These measurements provide new reaction rate coefficients for the ethynyl radical, C 2 H, with C 3 H 4 unsaturated hydrocarbons. These are necessary to extend current photochemical models of Jupiter, Saturn, and its satellite Titan.
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Molecular theory of gases and liquids
Robert L. Scott · Journal of Chemical Education · 1955 · 3.9K citations
Photochemical Modeling of Titan's Atmosphere
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Hydrocarbon Photochemistry in the Upper Atmosphere of Jupiter
G. R. Gladstone, M. Allen, Yuk L. Yung · Icarus · 1996 · 279 citations