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Published March 2009 | Published + Supplemental Material
Journal Article Open

Chemical mechanism for high temperature combustion of engine relevant fuels with emphasis on soot precursors

Abstract

This article presents a chemical mechanism for the high temperature combustion of a wide range of hydrocarbon fuels ranging from methane to iso-octane. The emphasis is placed on developing an accurate model for the formation of soot precursors for realistic fuel surrogates for premixed and diffusion flames. Species like acetylene (C_2H_2), propyne (C_3H_4), propene (C_3H_6), and butadiene (C_4H_6) play a major role in the formation of soot as their decomposition leads to the production of radicals involved in the formation of Polycyclic Aromatic Hydrocarbons (PAH) and the further growth of soot particles. A chemical kinetic mechanism is developed to represent the combustion of these molecules and is validated against a series of experimental data sets including laminar burning velocities and ignition delay times. To correctly predict the formation of soot precursors from the combustion of engine relevant fuels, additional species should be considered. One normal alkane (n-heptane), one ramified alkane (iso-octane), and two aromatics (benzene and toluene) were chosen as chemical species representative of the components typically found in these fuels. A sub-mechanism for the combustion of these four species has been added, and the full mechanism has been further validated. Finally, the mechanism is supplemented with a sub-mechanism for the formation of larger PAH molecules up to cyclo[cd]pyrene. Laminar premixed and counterflow diffusion flames are simulated to assess the ability of the mechanism to predict the formation of soot precursors in flames. The final mechanism contains 149 species and 1651 reactions (forward and backward reactions counted separately). The mechanism is available with thermodynamic and transport properties as supplemental material.

Additional Information

Copyright © 2008 The Combustion Institute. Received 12 February 2008; revised 5 December 2008; accepted 6 December 2008. Available online 17 January 2009. The authors gratefully acknowledge funding by the US Department of Energy within the ASC program, from SERDP, and from the Air Force Office of Scientific Research.

Attached Files

Published - mmc4.txt

Supplemental Material - mmc1.pdf

Supplemental Material - mmc2.txt

Supplemental Material - mmc3.txt

Supplemental Material - mmc5.txt

Supplemental Material - mmc6.txt

Supplemental Material - mmc7.txt

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Additional details

Created:
August 21, 2023
Modified:
October 19, 2023