Effect of pressure on soot formation in the pyrolysis of n-hexane and the oxidation of fuel-rich mixtures of n-heptane behind reflected shock waves
- Authors: Vlasov P.A.1,2, Smirnov V.N.1, Tereza A.M.1, Agafonov G.L.1, Kolbanovskii Y.A.3, Bilera I.V.3, Mihailov D.I.2, Zhil’tsova I.V.1
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Affiliations:
- Semenov Institute of Chemical Physics
- National Research Nuclear University MEPhI
- Topchiev Institute of Petrochemical Synthesis
- Issue: Vol 10, No 6 (2016)
- Pages: 912-921
- Section: Kinetics and Mechanism of Chemical Reactions. Catalysis
- URL: https://journal-vniispk.ru/1990-7931/article/view/198238
- DOI: https://doi.org/10.1134/S1990793116060282
- ID: 198238
Cite item
Abstract
The results of detailed kinetic simulations of the formation of soot particles in the pyrolysis of n-hexane–argon mixtures and in the oxidation of fuel-rich (φ = 5) n-heptane–oxygen–argon mixtures behind reflected shock waves at pressures of 20–100 bar and a constant concentration of carbon atoms or a constant fraction of argon in the initial mixture within the framework of a modified reaction mechanism are reported. The choice of n-hexane and n-heptane for examining the effect of pressure on the process of soot formation was motivated by the availability for these hydrocarbons of experimental measurements in reflected shock waves at high pressures (up to ~100 bar). The temperature dependences of the yield of soot particles formed in the pyrolysis of n-hexane are found to be very weakly dependent on pressure and slightly shifting to lower temperatures with increasing pressure. In general, pressure produces a very weak effect on the soot formation in the pyrolysis of n-hexane. The effect of pressure and concentration of carbon atoms in the initial mixture on the process of soot formation during the oxidation of fuel-rich n-heptane mixtures behind reflected shock waves is studied. The results of our kinetic simulations show that, for both the pyrolysis of n-hexane and the oxidation of fuel-rich n-heptane–oxygen mixtures, the influence of pressure on the process of soot formation is negligible. By contrast, the concentration of carbon atoms in the initial reaction mixture produces a much more pronounced effect.
About the authors
P. A. Vlasov
Semenov Institute of Chemical Physics; National Research Nuclear University MEPhI
Author for correspondence.
Email: iz@chph.ras.ru
Russian Federation, Moscow, 119991; Moscow, 115409
V. N. Smirnov
Semenov Institute of Chemical Physics
Email: iz@chph.ras.ru
Russian Federation, Moscow, 119991
A. M. Tereza
Semenov Institute of Chemical Physics
Email: iz@chph.ras.ru
Russian Federation, Moscow, 119991
G. L. Agafonov
Semenov Institute of Chemical Physics
Email: iz@chph.ras.ru
Russian Federation, Moscow, 119991
Yu. A. Kolbanovskii
Topchiev Institute of Petrochemical Synthesis
Email: iz@chph.ras.ru
Russian Federation, Moscow, 119991
I. V. Bilera
Topchiev Institute of Petrochemical Synthesis
Email: iz@chph.ras.ru
Russian Federation, Moscow, 119991
D. I. Mihailov
National Research Nuclear University MEPhI
Email: iz@chph.ras.ru
Russian Federation, Moscow, 115409
I. V. Zhil’tsova
Semenov Institute of Chemical Physics
Email: iz@chph.ras.ru
Russian Federation, Moscow, 119991
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