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首页> 外文期刊>Faraday discussions >An experimental and theoretical investigation of the competition between chemical reaction and relaxation for the reactions of ~1CH_2 with acetylene and ethene: implications for the chemistry of the giant planets
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An experimental and theoretical investigation of the competition between chemical reaction and relaxation for the reactions of ~1CH_2 with acetylene and ethene: implications for the chemistry of the giant planets

机译:〜1CH_2与乙炔和乙烯反应的化学反应与弛豫之间竞争的实验和理论研究:对巨型行星化学的影响

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摘要

The temperature dependence of the branching ratios for H atom production from the reactions of the first excited state of methylene (a~1A_1 ~1CH_2) with acetylene and ethene have been measured at 1 Torr total pressure and temperatures of 195, 250 and 298 K by monitoring the production of H atoms using laser induced fluorescence, comparing the signal to that observed from a calibration reaction. For the reaction with acetylene the yield of H increases from 0.28 (195 K) to 0.53 (250 K) to 0.88 at 298 K. The H atom yield from the reaction of ~1CH_2 with ethene shows similar behaviour, the yields being 0.35 (195 K), 0.51 (250 K) and 0.71 (298 K). The co-products, propargyl (C_3H_3) and allyl (C_3H_5) are formed from the dissociation of chemically activated C_3H_4 and C_3H_6 intermediates respectively, and are important species in the formation of higher hydrocarbons, including benzene, in the atmospheres of the outer planets and Titan. H atom production is in competition with electronic relaxation to form ground state methylene (X~3B_1, ~3CH_2) and collisional stabilization to form C_3H_4 and C_3H_6. Master equation calculations have been carried out to demonstrate that for the reaction of ~1CH_2 with acetylene, collisional stabilization is insignificant under experimental conditions and hence the balance of reaction is due to electronic relaxation. Non-adiabatic transition state theory has been applied to the reaction of ~1CH_2 with acetylene. The calculations show reasonable agreement with experiment, generally being within the combined errors, and reproduce the negative temperature dependence for electronic relaxation. The implications of the temperature dependence of the absolute rate coefficients for ~1CH_2 reactions with inert gases, hydrogen, acetylene and ethene and of the branching ratios between chemical reaction and electronic relaxation are discussed.
机译:在1 Torr总压力和195、250和298 K的温度下,测量了亚甲基的第一激发态(a〜1A_1〜1CH_2)与乙炔和乙烯反应生成H原子的支化比的温度依赖性。使用激光诱导的荧光监测H原子的产生,并将信号与从校准反应中观察到的信号进行比较。对于与乙炔的反应,H的产率在298 K时从0.28(195 K)增加到0.53(250 K)到0.88。〜1CH_2与乙烯反应的H原子产率表现出相似的行为,产率为0.35(195 K),0.51(250 K)和0.71(298 K)。副产物炔丙基(C_3H_3)和烯丙基(C_3H_5)分别是由化学活化的C_3H_4和C_3H_6中间体分解而形成的,它们是在外行星和大气中形成高级烃(包括苯)的重要物种。泰坦H原子的产生与电子弛豫形成基态亚甲基(X〜3B_1,〜3CH_2)和碰撞稳定形成C_3H_4和C_3H_6竞争。已经进行了主方程计算,以证明对于〜1CH_2与乙炔的反应,在实验条件下碰撞稳定作用不重要,因此反应的平衡归因于电子弛豫。非绝热过渡态理论已应用于〜1CH_2与乙炔的反应。计算结果与实验结果吻合合理,通常在组合误差范围内,并且再现了电子弛豫的负温度依赖性。讨论了与惰性气体,氢气,乙炔和乙烯进行的〜1CH_2反应的绝对速率系数的温度依赖性以及化学反应和电子弛豫之间的支化比的影响。

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