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COMPLETE BRANCHING RATIOS FOR THE DISSOCIATIVE RECOMBINATION OF H_2O~+, H_3O~+, AND CH_3~+

机译:H_2O〜+,H_3O〜+和CH_3〜+的解离重组的完全分支比

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摘要

Dissociative recombination of the polyatomic ions H_2O~+, H_3O~+, and CH_3~+ with electrons has been measured at the heavy-ion storage ring ASTRID. Complete branching ratios for all the possible product channels have been determined at zero relative energy using an energy-sensitive detector masked by grids with known transmissions. In the dissociative recombination of H_3O~+, water molecules are produced with a probability of 33%, whereas the production of atomic oxygen is negligible. Atomic carbon is, on the other hand, produced with a branching ratio of 30% in the dissociative recombination of CH_3~+. For all three molecular ions, the three-particle breakup is a major process. Relative cross sections for dissociative recombination of H_3O~+ and for dissociative excitation of H_3O~+ have been measured for relative electron energies up to 40 eV. Implications for the modeling of the chemistry of interstellar molecular clouds are discussed.
机译:在重离子存储环ASTRID处测量了多原子离子H_2O〜+,H_3O〜+和CH_3〜+与电子的解离重组。已经使用能量敏感的检测器确定了所有可能的产品通道的完全分支比,相对能量为零,该检测器被具有已知透射率的网格掩盖。在H_3O〜+的解离重组中,水分子的产生概率为33%,而原子氧的产生可以忽略不计。另一方面,在CH_3〜+的解离重组中,以30%的支化率产生原子碳。对于所有三个分子离子,三粒子破碎是一个主要过程。 H_3O〜+的解离重组和H_3O〜+的解离激发的相对截面已经测量到相对电子能量高达40 eV。讨论了星际分子云化学建模的意义。

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