Formation of nuclei and soot particles is computed following the empirical models of Tesner et al. [45]. The source terms are formulated in terms of particle number concentrations for nuclei:
(7–140) |
and soot particles:
(7–141) |
Where [part/mol]
is Avogadro’s number and:
(7–142) |
is the mass of a soot particle and
are the density and the mean diameter
of the soot particles, respectively. With the above definitions, the
source terms for nuclei
and soot formation
can be modeled as (Tesner et al. [45]):
(7–143) |
(7–144) |
In the nuclei equation, the spontaneous formation of radical
nuclei from the fuel, , is modeled using the Arrhenius approach,
(7–145) |
where is the mass fraction
of carbon in the fuel material.
is a linear branching coefficient,
is a linear
termination coefficient, and
is a coefficient of linear termination or radical
nuclei on soot particles. In the soot equation,
and
are constants.
The default values for all of the soot model parameters are summarized
in the following table:
Parameter |
Default Value by [part] |
Default value by [mol] |
---|---|---|
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|
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|
|
|
|
|
|
|
Fuel dependent (methane 12/16, acetylene 24/26) |
Fuel dependent (methane 12/16, acetylene 24/26) |
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
Most references list the coefficients using the absolute particle
number [part] in the physical dimensions. However, for numerical,
reasons CFX is using [mol] instead. To convert from the [part]
system into the [mol] system, coefficients and
have to
be multiplied by Avogadro’s number
[part/mol],
and the coefficient
must be divided by
. All other coefficients
remain unchanged.