Isomer-specific product detection of CN radical reactions with ethene and propene by tunable VUV photoionization mass spectrometry

被引:34
作者
Trevitt, Adam J. [1 ,2 ,3 ]
Goulay, Fabien [4 ]
Meloni, Giovanni [4 ]
Osborn, David L. [4 ]
Taatjes, Craig A. [4 ]
Leone, Stephen R. [1 ,2 ,3 ]
机构
[1] Univ Calif Berkeley, Dept Chem, Berkeley, CA 94720 USA
[2] Univ Calif Berkeley, Dept Phys, Berkeley, CA 94720 USA
[3] Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Berkeley, CA 94720 USA
[4] Sandia Natl Labs, Combust Res Facil, Livermore, CA 94551 USA
基金
美国国家航空航天局;
关键词
Product detection; CN radical; Alkenes; Synchrotron; Titan; SET MODEL CHEMISTRY; CROSS-SECTIONS; CYANO RADICALS; RATE CONSTANTS; HAZE FORMATION; SPECTROSCOPY; PRESSURE; VINYL; C2H2; (2)SIGMA(+));
D O I
10.1016/j.ijms.2008.07.033
中图分类号
O64 [物理化学(理论化学)、化学物理学]; O56 [分子物理学、原子物理学];
学科分类号
070203 ; 070304 ; 081704 ; 1406 ;
摘要
Product detection studies of CN reactions with ethene and propene are conducted at room temperature (41Torr, 533.3 Pa) using multiplexed time-resolved mass spectrometry with tunable synchrotron photoionization. Photoionization efficiency curves, i.e., the ion signal as a function of photon energy, are used to determine the products and distinguish isomers. Both reactions proceed predominantly via CN addition to the pi orbital of the olefin. For CN+ethene, cyanoethene (C2H3CN) is detected as the sole product in agreement with recent studies on this reaction. Multiple products are identified for the CN+ propene reaction with 75(+15)% of the detected products in the form of cyanoethene from a CH3 elimination channel and 25(+/- 15)% forming different isomers of C4H5N via H elimination. The C4H5N comprises 57(+15)% 1-cyanopropene, 43(+/- 15)% 2-cyanopropene and <15% 3-cyanopropene. No evidence of direct H abstraction or indirect HCN formation is detected for either reaction. The results have relevance to the molecular weight growth chemistry on Saturn's largest moon Titan, where the formation of small unsaturated nitriles are proposed to be key steps in the early chemical stages of haze formation. (C) 2008 Elsevier B.V. All rights reserved.
引用
收藏
页码:113 / 118
页数:6
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