高温下H + N2O和NH + NO反应激发OH生成动力学

IF 2.8 2区 化学 Q3 CHEMISTRY, PHYSICAL
Akira Matsugi*, 
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引用次数: 0

摘要

在含氮化合物燃烧过程中,提出了H + N2O→N2 + OH* (R1)和NH + NO→N2 + OH* (R2)反应是电子激发OH(A2Σ+)自由基的来源,表示为OH*。本研究通过激波管氢氧根发射实验研究了这些反应的动力学。利用动力学模拟分析了几种激波加热混合物中OH*浓度的时间分布。R1的速率常数由H2/N2O/Ar、NH3/N2O/Ar和C2H5I/N2O/Ar混合物的谱图确定,在T = 1600-2200 K的温度范围内,可以表示为k1 =(8.4±3.8)× 10-11 exp(-22900 K/T) cm3分子-1 s-1。对于R2,速率常数由NH3/NO/Ar和NH3/N2O/NO/Ar混合物的测量得到,表示为k2 =(1.6±0.8)× 10-13 exp(-10040 K/T) cm3分子-1 s-1在2000-2600 K范围内。根据速率常数的比较,讨论了OH*形成的可能机理。
本文章由计算机程序翻译,如有差异,请以英文原文为准。

Kinetics of Excited OH Formation in H + N2O and NH + NO Reactions at High Temperatures

Kinetics of Excited OH Formation in H + N2O and NH + NO Reactions at High Temperatures

The reactions H + N2O → N2 + OH* (R1) and NH + NO → N2 + OH* (R2) have been proposed as sources of the electronically excited OH(A2Σ+) radicals, denoted as OH*, during combustion of nitrogen-containing compounds. The present study investigates the kinetics of these reactions through OH* emission experiments using a shock tube. Time profiles of OH* concentration measured for several shock-heated mixtures are analyzed with the help of kinetic simulations. The rate constants for R1 are determined using the profiles obtained from H2/N2O/Ar, NH3/N2O/Ar, and C2H5I/N2O/Ar mixtures and can be expressed as k1 = (8.4 ± 3.8) × 10–11 exp(−22900 K/T) cm3 molecule–1 s–1 over the temperature range of T = 1600–2200 K. For R2, the rate constants are obtained from the measurements for NH3/NO/Ar and NH3/N2O/NO/Ar mixtures and are represented as k2 = (1.6 ± 0.8) × 10–13 exp(−10040 K/T) cm3 molecule–1 s–1 over 2000–2600 K. Possible mechanisms for the formation of OH* are discussed based on a comparison of the rate constants.

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来源期刊
The Journal of Physical Chemistry A
The Journal of Physical Chemistry A 化学-物理:原子、分子和化学物理
CiteScore
5.20
自引率
10.30%
发文量
922
审稿时长
1.3 months
期刊介绍: The Journal of Physical Chemistry A is devoted to reporting new and original experimental and theoretical basic research of interest to physical chemists, biophysical chemists, and chemical physicists.
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