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11.4 The Eulerian Solution Method

The Lagrangian solution method solves the composition PDF transport equation by stochastically tracking Lagrangian particles through the domain. It is computationally expensive since a large number of particles are required to represent the PDF, and a large number of iterations are necessary to reduce statistical errors and explicitly convect the particles through the domain. The Eulerian PDF transport model overcomes these limitations by assuming a shape for the PDF, which allows Eulerian transport equations to be derived. Stochastic errors are eliminated and the transport equations are solved implicitly, which is computationally economical. The multi-dimensional PDF shape is assumed as a product of delta functions. As with the Lagrangian PDF model, the highly non-linear chemical source term is closed. However, the turbulent scalar flux and molecular mixing terms must be modeled, and are closed with the gradient diffusion and the IEM models, respectively.

The composition PDF of $N_s + 1$ dimension ( $N_s$ species and enthalpy) is represented as a collection of $N_e$ delta functions (or modes). This presumed PDF has the following form:


 P(\psi;\vec{x},t) = \sum_{n=1}^{N_e} p_n(\vec{x},t) \prod_{k=1}^{N_s} \delta[\psi_k - <\phi_k>_n (\vec{x},t)] (11.4-1)

where $p_n$ is the probability in each mode, $<\phi_k>_n$ is the conditional mean composition of specie $k$ in the $n$th mode, $\psi_k$ is the composition space variable of specie $k$, and $\delta(\dots)$ is the delta function.

The Eulerian PDF transport equations are derived by substituting Equation  11.4-1 into the closed composition PDF transport equation (Equation  11.2-1 with Equations  11.2-2 and 11.3-6). The unknown terms, $p_n$ and $<\phi_k>_n$, are determined by forcing lower moments of this transported PDF to match the RANS lower moment transport equations, using the Direct Quadrature Method of Moments (DQMOM) approach [ 103, 218]. The resulting transport equations are:

where $p_n$ is the probability of the $n$th mode, and $s_{k,n} = p_n <\phi_k>_n$ is the $k$th specie probability weighted conditional mean composition of the $n$th mode. $\Gamma = \mu_l+\mu_t/{{\rm Sc}_t}$ is the effective turbulent diffusivity. The terms $M_{k,n}$, $S_{k,n}$ and $C_{k,n}$ represent mixing, reaction and correction terms respectively. Note that only $N_e-1$ probability equations are solved and the $N$th probability is calculated as one minus the sum of the $N_e-1$ solved probabilities.

Reaction

The reaction source term $S_{k,n}$ in Equation  11.4-3 for the $k$th composition and the $n$th mode is calculated as,


 S_{k,n} = p_n S(<\phi_k>_n )_k (11.4-4)

where $S()_k$ is the net reaction rate for the $k$th component.

Mixing

The micro-mixing term $M_{k,n}$ is modeled with the IEM mixing model:


 M_{k,n} = \frac{C_\phi}{\tau}(<\phi_k>_n - \psi_k) (11.4-5)

where $\tau$ is the turbulence time-scale and $C_\phi$ is the mixing constant.

Hence, for the two-mode DQMOM-IEM model, the mixing terms for component $k$ are,


$\displaystyle M_{k,1}$ $\textstyle =$ $\displaystyle \frac{C_\phi}{\tau}(p_1 s_{k,2} - p_2 s_{k,1} )$  
$\displaystyle M_{k,2}$ $\textstyle =$ $\displaystyle \frac{C_\phi}{\tau}(p_2 s_{k,1} - p_1 s_{k,2} )$ (11.4-6)

The default value of $C_\phi$ is 2, which is appropriate for gas-phase combustion. For reactions in liquids, where the diffusivities are much smaller than gases, the Liquid Micro-Mixing option interpolates $C_{\phi}$ from model turbulence [ 278] and scalar [ 103] spectra.

Correction

Using assumptions to ensure realizability and boundedness, the correction terms $C_{k,n}$ in Equation  11.4-3 for the $k$th composition are determined from the linear system,


 \sum_{n=1}^{N_e} <\phi_k>_n^{m_k - 1} C_{k,n} = \sum_{n=1}^{N_e}(m_k - 1)<\phi_k>_n^{m_k - 2} p_n c_{k,n} (11.4-7)

where $m_k$ are the non-negative integer lower moments (1.. $N_e$) for each component $k$. Note that the condition of the matrix decreases with increasing $m_k$, which reduces the stability of higher mode simulations.

The dissipation term $c_{k,n}$ in Equation  11.4-7 is calculated as,


 c_{k,n} = \Gamma \nabla(<\phi_k>_n ) \cdot \nabla(<\phi_k>_n ) (11.4-8)

For the two-mode DQMOM-IEM model, the correction terms for the $k$th component are,


$\displaystyle C_{k,1}$ $\textstyle =$ $\displaystyle \frac{\Gamma}{<\phi_k>_1-<\phi_k>_2} \left(p_1 (\nabla <\phi_k>_1 )^2 + p_2 (\nabla <\phi_k>_2 )^2 \right)$  
$\displaystyle C_{k,2}$ $\textstyle =$ $\displaystyle -C_{k,1}$ (11.4-9)

Calculation of Composition Mean and Variance

The mean composition (specie $k$ or energy) is calculated as,


 \overline{\phi_k} = \sum_{n=1}^{N_e} {s_{k,n}} (11.4-10)

and its variance is calculated as


 \overline{\phi_k^{'2}} = (\sum_{n=1}^{N_e} {s_{k,n} <\phi_k>_n}) - \overline{\phi_k}^2 (11.4-11)


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