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首页> 外文期刊>The Journal of Chemical Physics >Metastable hydronium ions in UV-irradiated ice
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Metastable hydronium ions in UV-irradiated ice

机译:紫外线辐射的冰中的亚稳态水合氢离子

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We show that the irradiation of UV light (10-11 eV) onto an ice film produces metastable hydronium (H_3O~+) ions in the ice at low temperatures (53-140 K). Evidence of the presence of metastable hydronium ions was obtained by experiments involving adsorption of methylamine onto UV-irradiated ice films and hydrogen-deuterium (HD) isotopic exchange reaction. The methylamine adsorption experiments showed that photogenerated H _3O~+ species transferred a proton to the methylamine arriving at the ice surface, thus producing the methyl ammonium ion, which was detected by low energy sputtering method. The H_3O~+ species induced the HD exchange of water, which was monitored through the detection of water isotopomers on the surface by using the Cs~+ reactive ion scattering method. Thermal and temporal stabilities of H3O + and its proton migration activity were examined. The lifetime of the hydronium ions in the amorphized ice was greater than 1 h at ~53 K and decreased to ~5 min at 140 K. Interestingly, a small portion of hydronium ions survived for an extraordinarily long time in the ice, even at 140 K. The average migration distance of protons released from H_3O~+ in the ice was estimated to be about two water molecules at ~54 K and about six molecules at 100 K. These results indicate that UV-generated hydronium ions can be efficiently stabilized in low-temperature ice. Such metastable hydronium ions may play a significant role in the acid-base chemistry of ice particles in interstellar clouds.
机译:我们表明,紫外线(10-11 eV)照射到冰膜上时,在低温(53-140 K)下的冰中产生亚稳态的水合氢(H_3O〜+)离子。通过涉及将甲胺吸附到紫外线辐射的冰膜上以及氢-氘(HD)同位素交换反应的实验获得了亚稳氢离子的存在的证据。甲胺的吸附实验表明,光生H _3O〜+物质将质子转移到到达冰面的甲胺上,从而产生了甲基铵离子,该离子可通过低能溅射法检测到。 H_3O〜+物种引起水的高清交换,通过使用Cs〜+反应离子散射法检测表面上的水同位素异构体来监测。研究了H3O +的热和时间稳定性及其质子迁移活性。非晶态冰中水合氢离子的寿命在〜53 K时大于1小时,在140 K时降低至〜5分钟。有趣的是,即使在140 K时,一小部分水合氢离子在冰中的存活时间也非常长。从H_3O〜+释放的质子在冰中的平均迁移距离估计为约54 K时约2个水分子和100 K时约6个水分子。这些结果表明,紫外线产生的水合氢离子可在低温冰。这种亚稳定的水合氢离子可能在星际云中冰粒的酸碱化学中起重要作用。

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