首页> 外文期刊>The journal of physical chemistry, A. Molecules, spectroscopy, kinetics, environment, & general theory >248-nm laser photolysis of CHBr3/O-atom mixtures: Kinetic evidence for UVCO(A) chemiluminescence in the reaction of methylidyne radicals with atomic oxygen
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248-nm laser photolysis of CHBr3/O-atom mixtures: Kinetic evidence for UVCO(A) chemiluminescence in the reaction of methylidyne radicals with atomic oxygen

机译:CHBr3 / O原子混合物的248 nm激光光解:亚甲基自由基与原子氧反应中UVCO(A)化学发光的动力学证据

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The 4th positive and Cameron band emissions from electronically excited CO have been observed for the first time in 248-nm pulsed laser photolysis of a trace amount of CHBr3 vapor in an excess of O atoms. O atoms were produced by dissociation of N2O (or O-2) in a cw-microwave discharge cavity in 2.0 Torr of He at 298 K. The CO emission intensity in these bands showed a quadratic dependence on the laser fluence employed. Temporal profiles of the CO(A) and other excited-state products that formed in the photoproduced precursor + O-atom reactions were measured by recording their time-resolved chemiluminescence in discrete vibronic bands. The CO 4th positive transition (A(1)Pi, v' = 0 -> X(1)Sigma(+), v'' = 2) near 165.7 nm was monitored in this work to deduce the pseudo-first-order decay kinetics of the CO(A) chemiluminescence in the presence of various added substrates (CH4, NO, N2O, H-2, and O-2). From this, the second-order rate coefficient values were determined for reactions of these substrates with the photoproduced precursors. The measured reactivity trends suggest that the prominent precursors responsible for the CO(A) chemiluminescence are the methylidyne radicals, CH(X(2)Pi) and CH(a(4)Sigma(-)), whose production requires the absorption of at least 2 laser photons by the photolysis mixture. The O-atorn reactions with brominated precursors (CBr, CHBr, and CBr2), which also form in the photolysis, are shown to play a minor role in the production of the CO(A or a) chemiluminescence. However, the CBr2 + O-atom reaction was identified as a significant source for the 289.9-nm Br-2 chemiluminescence that was also observed in this work. The 282.2-nm OH and the 336.2-nm NH chemiluminescences were also monitored to deduce the kinetics of CH(X(2)Pi) and CH(a(4)Sigma(-)) reactions when excess O-2 and NO were present.
机译:在248 nm脉冲激光光解中,在过量O原子中的痕量CHBr3蒸气中,首次观察到了来自电子激发的CO的第四正带和Cameron带发射。 O原子是通过在298 K的He下2.0 Torr的连续波微波放电腔中分解N2O(或O-2)而产生的。这些波段中的CO发射强度对所使用的激光通量呈二次依赖性。通过在离散的电子束带中记录时间分辨的化学发光来测量在光生前体+ O原子反应中形成的CO(A)和其他激发态产物的时间分布。在这项工作中监测了接近165.7 nm的CO第四正跃迁(A(1)Pi,v'= 0-> X(1)Sigma(+),v''= 2)以推导伪一阶衰减各种添加底物(CH4,NO,N2O,H-2和O-2)存在下CO(A)化学发光的动力学。由此,确定这些基板与光生前体的反应的二阶速率系数值。测得的反应趋势表明,负责CO(A)化学发光的主要前体是亚甲基自由基,CH(X(2)Pi)和CH(a(4)Sigma(-)),其产生需要吸收光解混合物至少产生2个激光光子。与溴化前体(CBr,CHBr和CBr2)的O-atorn反应(也在光解过程中形成)显示在CO(A或a)化学发光的产生中起次要作用。但是,CBr2 + O原子反应被认为是289.9 nm Br-2化学发光的重要来源,在这项工作中也观察到了这一现象。还监测了282.2 nm的OH和336.2 nm的NH化学发光,以推断存在过量O-2和NO时CH(X(2)Pi)和CH(a(4)Sigma(-))反应的动力学。 。

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