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首页> 外文期刊>The Astrophysical journal >FORMATION OF KETENE (H2CCO) IN INTERSTELLAR ANALOGOUS METHANE (CH4)-CARBON MONOXIDE (CO) ICES: A COMBINED FTIR AND REFLECTRON TIME-OF-FLIGHT MASS SPECTROSCOPIC STUDY
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FORMATION OF KETENE (H2CCO) IN INTERSTELLAR ANALOGOUS METHANE (CH4)-CARBON MONOXIDE (CO) ICES: A COMBINED FTIR AND REFLECTRON TIME-OF-FLIGHT MASS SPECTROSCOPIC STUDY

机译:星际间甲烷(CH4)-一氧化碳(CO)冰中酮(H2CCO)的形成:FTIR和反射电子飞行时间质谱的组合研究

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摘要

The formation of ketene (H2CCO) in methane-carbon monoxide (CH4-CO) ices was investigated upon its exposure to ionizing radiation in the form of energetic electrons at 5.5?K. The radiation-induced nonthermal equilibrium processing of these ices was monitored online and in situ via infrared spectroscopy complimented with post-irradiation temperature programmed desorption studies exploiting highly sensitive reflectron time-of-flight mass spectrometry (ReTOF) coupled with single photon fragment-free photo ionization (PI) at 10.49?eV. The detection of ketene in irradiated (isotopically labeled) methane-carbon monoxide ices was confirmed via the ν2 infrared absorption band and substantiated during the warm-up phase based on sublimation profiles obtained from the ReTOF-PI spectra of the corresponding isotopic masses. The experiments conducted with the mixed isotopic ices of 12CD4-13CO provide clear evidence of the formation of at least two ketene isotopomers (D2 12C13CO and D2 13C13CO), allowing for the derivation of two competing formation pathways. We have also proposed underlying reaction mechanisms to the formation of ketene based on kinetic fitting of the temporal evolution of the ketene isotopomers.
机译:研究了甲烷-一氧化碳(CH4-CO)冰中乙烯酮(H2CCO)的形成,该过程以5.5?K的高能电子形式暴露于电离辐射中。这些冰的辐射诱导的非热平衡过程可通过红外光谱进行在线和原位监测,并辅以利用高灵敏度反射电子飞行时间质谱(ReTOF)和无单光子碎片照片的辐照后程序升温解吸研究电离(PI)为10.49?eV。通过ν2红外吸收带确认了在辐照的(同位素标记的)甲烷-一氧化碳冰中的乙烯酮的检测,并在预热阶段根据从相应同位素质量的ReTOF-PI光谱获得的升华曲线进行了证实。用12CD4-13CO的混合同位素冰进行的实验提供了至少两种烯酮异构体(D2 12C13CO和D2 13C13CO)形成的清晰证据,从而可以推导两个竞争的形成途径。我们还提出了基于乙烯酮异位异构体随时间变化的动力学拟合而对乙烯酮形成的基本反应机理。

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