FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W2902470939> ?p ?o ?g. }

• W2902470939 endingPage "49" @default.
• W2902470939 startingPage "34" @default.
• W2902470939 abstract "Several method of moments (MOM) models were developed recently to describe the evolution of soot particle populations. However, especially soot oxidation is still very challenging in MOM, as pointwise information of the underlying soot particle number density function (NDF) is usually unknown and thus, the prediction of smallest particles that oxidize completely is not easy. The recently proposed Extended Quadrature Method of Moments (EQMOM) (Yuan, Laurent, & Fox, 2012) has the potential to resolve this issue providing a continuous NDF reconstruction based on the set of transported moments. While its general suitability for soot was already demonstrated in the literature, the EQMOM moment inversion procedure reveals several numerical difficulties. In this work, we propose an EQMOM modification called split-based EQMOM that builds upon the general idea of EQMOM to represent the NDF by a weighted sum of superimposed, non-negative, continuous kernel density functions (KDFs), avoiding, however, the numerical problems of its original version. The model is based on a split of the entire NDF into a sum of overlaying density functions, whose evolution is governed by individual population balance equations (PBEs). These PBEs are derived and implemented in a novel Monte Carlo (MC) framework which is applied to simulate two fuel-rich burner-stabilized laminar premixed flames with different sooting behaviours. Results are compared to a classical MC model to demonstrate the suitability. Next, the MC data is used to assess the suitability of lognormal, gamma and inverse Gaussian distributions to approximate the NDF shape by employing the Wasserstein metric as criterion. This information is finally used to formulate an improved EQMOM soot model, which is then evaluated for both fuel-rich and oxidizing conditions. For the latter, the two-stage burner experiments of Echavarria, Jaramillo, Sarofim, & Lighty (2011) is considered, where particle oxidation is the dominant process. It is demonstrated that the proposed MOM model allows an accurate and numerically robust description of soot formation, growth and also oxidation." @default.
• W2902470939 created "2018-12-11" @default.
• W2902470939 creator A5018895376 @default.
• W2902470939 creator A5034190951 @default.
• W2902470939 creator A5074713766 @default.
• W2902470939 creator A5080730496 @default.
• W2902470939 date "2019-02-01" @default.
• W2902470939 modified "2023-10-18" @default.
• W2902470939 title "A numerically robust method of moments with number density function reconstruction and its application to soot formation, growth and oxidation" @default.
• W2902470939 cites W1966281189 @default.
• W2902470939 cites W1970235890 @default.
• W2902470939 cites W1971818437 @default.
• W2902470939 cites W1974442389 @default.
• W2902470939 cites W1974675482 @default.
• W2902470939 cites W1975207767 @default.
• W2902470939 cites W1978886093 @default.
• W2902470939 cites W1986271190 @default.
• W2902470939 cites W1992253067 @default.
• W2902470939 cites W1993963907 @default.
• W2902470939 cites W2000809527 @default.
• W2902470939 cites W2005981060 @default.
• W2902470939 cites W2008183064 @default.
• W2902470939 cites W2013423989 @default.
• W2902470939 cites W2014142501 @default.
• W2902470939 cites W2014688420 @default.
• W2902470939 cites W2017822291 @default.
• W2902470939 cites W2020138725 @default.
• W2902470939 cites W2025376439 @default.
• W2902470939 cites W2039006687 @default.
• W2902470939 cites W2039391192 @default.
• W2902470939 cites W2044048010 @default.
• W2902470939 cites W2045128394 @default.
• W2902470939 cites W2045744723 @default.
• W2902470939 cites W2046281592 @default.
• W2902470939 cites W2047521014 @default.
• W2902470939 cites W2047810407 @default.
• W2902470939 cites W2049609957 @default.
• W2902470939 cites W2053360806 @default.
• W2902470939 cites W2053621873 @default.
• W2902470939 cites W2063078040 @default.
• W2902470939 cites W2063430114 @default.
• W2902470939 cites W2073263581 @default.
• W2902470939 cites W2073740326 @default.
• W2902470939 cites W2075230606 @default.
• W2902470939 cites W2076004235 @default.
• W2902470939 cites W2076192422 @default.
• W2902470939 cites W2079062813 @default.
• W2902470939 cites W2084388913 @default.
• W2902470939 cites W2084848231 @default.
• W2902470939 cites W2085079835 @default.
• W2902470939 cites W2085708866 @default.
• W2902470939 cites W2091802923 @default.
• W2902470939 cites W2147972077 @default.
• W2902470939 cites W2168939220 @default.
• W2902470939 cites W2170934473 @default.
• W2902470939 cites W2176253740 @default.
• W2902470939 cites W2191784405 @default.
• W2902470939 cites W2465532475 @default.
• W2902470939 cites W2519739338 @default.
• W2902470939 cites W2522680391 @default.
• W2902470939 cites W2583633986 @default.
• W2902470939 cites W2605564132 @default.
• W2902470939 cites W2783953982 @default.
• W2902470939 cites W2793119187 @default.
• W2902470939 cites W572419094 @default.
• W2902470939 doi "https://doi.org/10.1016/j.jaerosci.2018.11.009" @default.
• W2902470939 hasPublicationYear "2019" @default.
• W2902470939 type Work @default.
• W2902470939 sameAs 2902470939 @default.
• W2902470939 citedByCount "22" @default.
• W2902470939 countsByYear W29024709392019 @default.
• W2902470939 countsByYear W29024709392020 @default.
• W2902470939 countsByYear W29024709392021 @default.
• W2902470939 countsByYear W29024709392022 @default.
• W2902470939 countsByYear W29024709392023 @default.
• W2902470939 crossrefType "journal-article" @default.
• W2902470939 hasAuthorship W2902470939A5018895376 @default.
• W2902470939 hasAuthorship W2902470939A5034190951 @default.
• W2902470939 hasAuthorship W2902470939A5074713766 @default.
• W2902470939 hasAuthorship W2902470939A5080730496 @default.
• W2902470939 hasConcept C105795698 @default.
• W2902470939 hasConcept C105923489 @default.
• W2902470939 hasConcept C121332964 @default.
• W2902470939 hasConcept C121864883 @default.
• W2902470939 hasConcept C134306372 @default.
• W2902470939 hasConcept C151620405 @default.
• W2902470939 hasConcept C178790620 @default.
• W2902470939 hasConcept C179254644 @default.
• W2902470939 hasConcept C185592680 @default.
• W2902470939 hasConcept C19499675 @default.
• W2902470939 hasConcept C197055811 @default.
• W2902470939 hasConcept C2775925408 @default.
• W2902470939 hasConcept C2777634741 @default.
• W2902470939 hasConcept C2777984123 @default.
• W2902470939 hasConcept C28826006 @default.
• W2902470939 hasConcept C33923547 @default.
• W2902470939 hasConcept C74650414 @default.
• W2902470939 hasConceptScore W2902470939C105795698 @default.

• next