2010
DOI: 10.1016/j.combustflame.2009.11.013
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Modelling the internal structure of nascent soot particles

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Cited by 128 publications
(82 citation statements)
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References 32 publications
(44 reference statements)
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“…On-line ELPI and AE-33 (at 880 nm) measurements made it possible to investigate BC/PN and BC/PM 10 correlations. In order to quantify the black carbon fraction in total PM 10 particle mass, PM 10 was estimated from ELPI data assuming that the particles were spherical with a particle density of 1.2 g/cm 3 (Totton et al, 2010;Barone et al, 2011). The correlations between black carbon and particle number/mass emissions for Diesel and gasoline vehicles are presented in Fig.…”
Section: Pn Bc and No 2 Analysesmentioning
confidence: 99%
“…On-line ELPI and AE-33 (at 880 nm) measurements made it possible to investigate BC/PN and BC/PM 10 correlations. In order to quantify the black carbon fraction in total PM 10 particle mass, PM 10 was estimated from ELPI data assuming that the particles were spherical with a particle density of 1.2 g/cm 3 (Totton et al, 2010;Barone et al, 2011). The correlations between black carbon and particle number/mass emissions for Diesel and gasoline vehicles are presented in Fig.…”
Section: Pn Bc and No 2 Analysesmentioning
confidence: 99%
“…Even for mature soot, its properties are subject to large uncertainties (Michelsen et al 2007). Some attention has been paid to the mass density of young soot in several recent studies Camacho et al 2015;L opez-Yglesias et al 2014;Totton et al 2010). While Totton et al (2010) recommended a very low value of 1.12 g/cm 3 for incipient soot density, a higher value of 1.5 g/cm 3 was preferred by Zhao et al (2007) and Camacho et al (2015) for the density of newly formed incipient soot.…”
Section: Thermal and Optical Properties Of Incipient Sootmentioning
confidence: 99%
“…Some attention has been paid to the mass density of young soot in several recent studies Camacho et al 2015;L opez-Yglesias et al 2014;Totton et al 2010). While Totton et al (2010) recommended a very low value of 1.12 g/cm 3 for incipient soot density, a higher value of 1.5 g/cm 3 was preferred by Zhao et al (2007) and Camacho et al (2015) for the density of newly formed incipient soot. It is noticed that the value of 1.5 g/cm 3 seems more reasonable based on the consideration that the mass densities of soot precursors are around 1.3 g/cm 3 (1.27 g/cm 3 for pyrene and 1.35 g/cm 3 for benzopyrene).…”
Section: Thermal and Optical Properties Of Incipient Sootmentioning
confidence: 99%
“…Soot morphology has been studied numerically [27,48,62] and experimentally [22] for decades but understanding the processes that determine the morphology remains a very challenging and complex problem. Polycyclic aromatic hydrocarbons (PAHs) are often invoked as key precursors to soot formation [10,44,45].…”
Section: Introductionmentioning
confidence: 99%