2004
DOI: 10.1080/00102200490487544
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DETAILED KINETIC MODELING OF SOOT FORMATION DURING SHOCK-TUBE PYROLYSIS OF C6H6: DIRECT COMPARISON WITH THE RESULTS OF TIME-RESOLVED LASER-INDUCED INCANDESCENCE (LII) AND CW-LASER EXTINCTION MEASUREMENTS

Abstract: The results of calculations of the main parameters of the soot formation process (t, k f , SY, and r m ) carried out with the use of the detailed kinetic model of soot formation are compared with the experimental measurements of these parameters by the continuous-wave (CW)-laser extinction technique and by the time-resolved laser-induced incandescence (LII) method during C 6 H 6 pyrolysis behind reflected shock waves. The detailed kinetic model of soot formation that is developed incorporates the gas-phase mec… Show more

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Cited by 29 publications
(19 citation statements)
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“…The formation of light hydrocarbons by radical recombination reactions, with resulting products such as acetylene (C 2 H 2 ) and small olefins may be source to the formation of even heavier coke precursor species. Combination reactions of acetylene, and alternatively addition and dehydrogenation steps of small olefins like ethylene and propylene, may give rise to increasing concentration of aromatics (C 6 H 6 ) and polycyclic aromatic hydrocarbons (PAHs) which are also highly potent coke precursors. The consequences of these findings are fundamental in nature: not only is C1 related coke build‐up highly relevant, but even if present in much lower concentration in the feed, coke precursors like acetylene, small olefins and aromatics are present and any catalyst material will be subject to the consequences of their presence.…”
Section: Introductionmentioning
confidence: 99%
“…The formation of light hydrocarbons by radical recombination reactions, with resulting products such as acetylene (C 2 H 2 ) and small olefins may be source to the formation of even heavier coke precursor species. Combination reactions of acetylene, and alternatively addition and dehydrogenation steps of small olefins like ethylene and propylene, may give rise to increasing concentration of aromatics (C 6 H 6 ) and polycyclic aromatic hydrocarbons (PAHs) which are also highly potent coke precursors. The consequences of these findings are fundamental in nature: not only is C1 related coke build‐up highly relevant, but even if present in much lower concentration in the feed, coke precursors like acetylene, small olefins and aromatics are present and any catalyst material will be subject to the consequences of their presence.…”
Section: Introductionmentioning
confidence: 99%
“…They incorporated the mean value of fractal dimension into their model as well as the agglomerate collision diameter and the number of primary particles. Not using PARSIVAL or PREDICI but based on Wulkow's earlier work, Vlasov, Warnatz and co-workers employed a finite element code to simulate the formation of soot in a shock tube 119,80) .…”
Section: Finite Element Methodsmentioning
confidence: 99%
“…The majority of studies on soot formation concern shock-tube pyrolysis and laminar flame techniques. 5,6 There is considerable evidence that PAHs play a key role in soot formation, although other reaction pathways involving polyacetylenes and ionic species have been suggested. 82 There are several comprehensive reviews on the chemical pathways of soot formation; 4, 80, 81 generally four phases (P) in soot formation can be distinguished P1: The phase in which small molecular precursors to soot (such as small aromatic species like benzene or naphthalene) are either present or formed.…”
Section: B Considerations Regarding Particle Formationmentioning
confidence: 99%
“…The combination of the mutagenic and/or carcinogenic properties of many PAHs 1,2 and their efficient formation during the incomplete combustion of organic materials, has resulted in a large effort to understand the fundamental role of PAHs in combustion chemistry. 3,4 Hence, their physical and chemical properties have been extensively studied under a variety of environmentally relevant experimental conditions, e.g., in shock-tube pyrolysis 5,6 and flame combustion studies. 7,8 Due to their strong affinities to carbonaceous matter, such as coal or soot, the occurrence of PAHs in fine particulate matter in the atmosphere and their formation, e.g., in the context of black carbon particles, 9 is of significant interest in atmospheric/environmental sciences.…”
Section: Introductionmentioning
confidence: 99%