Atmospheric reactions Cl+CH3-(CH2)n-OH (n=0-4):: A kinetic and theoretical study

被引:33
|
作者
Garzon, Andres
Cuevas, Carlos A.
Ceacero, AntonAio A.
Notario, Alberto
Albaladejo, Jose
Fernandez-Gomez, Manuel
机构
[1] Univ Castilla La Mancha, Fac CC Quim, E-13071 Ciudad Real, Spain
[2] Univ Castilla La Mancha, ITQUIMA, E-13071 Ciudad Real, Spain
[3] Univ Jaen, Dept Quim Fis & Analit, Jaen 23071, Spain
来源
JOURNAL OF CHEMICAL PHYSICS | 2006年 / 125卷 / 10期
关键词
D O I
10.1063/1.2244556
中图分类号
O64 [物理化学(理论化学)、化学物理学];
学科分类号
070304 ; 081704 ;
摘要
The reactions of Cl with a series of linear alcohols: methanol (k(1)), ethanol (k(2)), 1-propanol (k(3)), 1-butanol (k(4)), and 1-pentanol (k(5)) were investigated as a function of temperature in the range of 264-382 K by laser photolysis-resonance fluorescence. The obtained kinetic data were used to derive the following Arrhenius expressions: k(1)=(3.55 +/- 0.22)x10(-10) exp[-(559 +/- 40)/T], k(2)=(5.25 +/- 0.52)x10(-11) exp[(190 +/- 68)/T], k(3)=(2.63 +/- 0.21)x10(-11) exp[(525 +/- 51)/T], k(4)=(3.12 +/- 0.31)x10(-11) exp[(548 +/- 65)/T], and k(5)=(3.97 +/- 0.48)x10(-11) exp[(533 +/- 77)/T] (in units of cm(3) molecule(-1) s(-1)). To our knowledge, these are the first absolute kinetic data reported for 1-butanol and 1-pentanol and also the first kinetic study as a function of temperature for these two compounds. Results, mechanism, and tropospheric implications are discussed and compared with the reported reactivity with OH radicals. Moreover, a theoretical insight into the mechanisms of these reactions has also been pursued through ab initio Moller-Plesset second-order perturbation treatment calculations with 6-311G(**) basis sets. Optimized geometries and vibrational frequencies have been obtained for transition states and molecular complexes appearing along the different reaction pathways. Furthermore, molecular energies have been calculated at quadratic configuration interaction with single, double, and triple excitations level in order to get an estimation of the activation energies. (c) 2006 American Institute of Physics.
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