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- W1999652934 abstract "Translationally hot (3.7 eV center-of-mass collision energy) D atoms can be produced by the dissociative recombinationsof DCO+ ions with electrons in interstellar clouds. The reactions of hot D atoms with H2 molecules is an important factor in determining the D to H abundance ratio in the universe from observations of deuterated species in dense interstellar clouds. A simulation of this reaction has been carried out using exact quasiclassical reaction cross sections, together with a series of approximate total collision cross sections. It was found that the total probability of reaction, PR, at 3.7 eV was approximately 0.4. A reaction probability of this magnitude suggeststhat the loss of D atoms by the title reaction be considered in astrochemical modeling of deuterated molecules." @default.
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- W1999652934 date "1986-09-01" @default.
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- W1999652934 title "Total reaction probabilities for translationally hot (3.7 eV)D atoms reacting with H2 and their astrophysical implications" @default.
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- W1999652934 doi "https://doi.org/10.1002/kin.550180908" @default.
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