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互不相溶物的混合:接近冰结晶温度时水中冰里的碳氢化合物

Mixing of the immiscible: hydrocarbons in water-ice near the ice crystallization temperature.

作者信息

Lignell Antti, Gudipati Murthy S

机构信息

Ice Spectroscopy Lab, Science Division, Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, California 91109, United States.

出版信息

J Phys Chem A. 2015 Mar 19;119(11):2607-13. doi: 10.1021/jp509513s. Epub 2014 Oct 27.

Abstract

Structural changes in hydrocarbon-doped water-ice during amorphous to crystalline phase conversion are investigated using polycyclic aromatic hydrocarbons (PAHs) as probes. We show that aggregation of impurity molecules occurs due to the amorphous-crystalline transition in ice, especially when they are hydrophobic molecules such as PAHs. Using ultraviolet-visible (UV-vis), Fourier-transform Infrared (FTIR), and laser-induced-fluorescence (LIF) spectroscopic techniques, we show that, although ice infrared absorption features change from a broad structureless band corresponding to amorphous ice to a sharp structured crystalline ice bands, simultaneously, sharper isolated PAH UV absorption features measured in the amorphous ice host turn broad upon ice crystallization. A simultaneous decrease in the monomer fluorescence and increase in the excimer emission band is observed, a clear indication for the formation of PAH molecular aggregates when amorphous ice is converted to crystalline ice at higher temperatures. Similar to the irreversible amorphous-crystalline phase transitions, the UV, fluorescence, and excimer emissions indicate that PAHs undergo irreversible aggregation. Our studies suggest that organic impurities exist as aggregates rather than monomers trapped in crystalline water-ice when cycled through temperatures that convert amorphous ice to crystalline ice, rendering a better insight into phenomena such as the formation of cometary crust. This aggregate formation also may significantly change the secondary reaction pathways and rates in impurity-doped ices in the lab, on Earth, in the solar system, and in the interstellar medium.

摘要

利用多环芳烃(PAHs)作为探针,研究了碳氢化合物掺杂水冰在非晶态到晶态转变过程中的结构变化。我们发现,由于冰中的非晶态-晶态转变,杂质分子会发生聚集,尤其是当它们是疏水分子(如PAHs)时。通过紫外-可见(UV-vis)、傅里叶变换红外(FTIR)和激光诱导荧光(LIF)光谱技术,我们发现,尽管冰的红外吸收特征从对应于非晶冰的宽无结构带变为尖锐的结构化晶冰带,但同时,在非晶冰主体中测量到的更尖锐的孤立PAH紫外吸收特征在冰结晶时会变宽。观察到单体荧光同时降低,准分子发射带增加,这清楚地表明当非晶冰在较高温度下转变为晶冰时,PAH分子聚集体形成。与不可逆的非晶态-晶态相变类似,紫外、荧光和准分子发射表明PAHs发生了不可逆聚集。我们的研究表明,当经历将非晶冰转变为晶冰的温度循环时,有机杂质以聚集体而非被困在晶态水冰中的单体形式存在,这有助于更好地理解彗星地壳形成等现象。这种聚集体的形成也可能显著改变实验室、地球上、太阳系和星际介质中杂质掺杂冰中的二级反应途径和速率。

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