NeuralFlowTheory & User Reference Manual
Carrier Flux Discretization on Interior Faces
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6 Carrier Flux Discretization on Interior Faces

6.1 Face geometry and orientation

Consider an interior face shared by cells and . The unit normal is oriented from to and the area is . A conservative numerical flux must satisfy the orientation identity (6.1) so that the same face contribution enters neighbouring cells with opposite sign.

Finite-volume control volume sketch
Figure 6.1: Finite-volume control volume and outward differential surface element used in the integral conservation statements.
Interior face geometry with left and right cells
Figure 6.2: Interior-face geometry with left and right cell locations used for flux reconstruction.

6.2 Compressible AUSM-family flux

For a compressible aerodynamic state, an AUSM-family inviscid face flux can be separated into a numerical mass flux and mechanical pressure, (6.2) with appended turbulence/species components transported by the appropriate numerical mass flux. AUSM+-up constructs from split Mach functions and a pressure-difference correction, and constructs from split pressure functions and a velocity-difference correction (Liou 2006). This separation is valuable for a primitive-variable coupled solver because pressure-to-continuity and velocity-to-momentum couplings appear directly in the face Jacobian.

For a moving/rotating coordinate representation the convective normal speed is formed relative to the grid/frame velocity. The energy flux must then be derived consistently for the selected absolute- or relative-energy formulation. The current NeuralFlow formulation status of this term is discussed in Chapter 20.

6.3 Constant-density artificial-compressibility flux

For the incompressible regime, the pressure-index row is the numerical mass flux rather than a density flux. The current row structure is (6.3) where is mass flux per unit area. Turbulence and species rows use the same . Because the physical density is constant, pressure influences continuity through the AUSM+-up pressure-difference correction and through the pseudo-time pressure coefficient, not through an equation-of-state derivative .

6.4 Viscous momentum flux

The viscous momentum flux is with from Eq. (2.4). On an unstructured cell-centred grid, is reconstructed at the face. For non-orthogonal grids a simple two-point normal difference is insufficient by itself; the reconstruction must retain the tangential/non-orthogonal gradient contribution used by the active NeuralFlow gradient path.

6.5 Energy and species diffusion

The viscous/thermal energy flux contains heat conduction and, where enabled, viscous work and species enthalpy diffusion, The exact active terms depend on solver options and material/species configuration. A dependent-species formulation requires the enthalpy-diffusion correction to be constructed consistently with Eq. (2.6).

6.6 AD face Jacobian

For each face, the complete expression is differentiated with respect to both cell states, For cell , these derivatives are accumulated into its diagonal and -neighbour matrix blocks. For cell , the same conservative face flux is assembled with opposite orientation. This produces the block-sparse nearest-neighbour coupling used by the global implicit solver.

6.7 HLLC carrier flux

The current compressible carrier solver also contains an HLLC flux path. NeuralFlow forms density-weighted Einfeldt-type left and right signal estimates. With face-normal velocities and , the Roe-like normal velocity and acoustic estimate are

The bounding wave speeds are and . The contact speed is determined from pressure and momentum continuity across the star region, and the final HLLC flux selects the left, left-star, right-star or right state according to the signs of , and . Species are convected with the selected mass flux. The homogeneous VOF production path currently uses the AUSM carrier flux rather than HLLC.

Writing the formulation wave estimates explicitly, with and ,

The contact-wave speed used by the current carrier HLLC path is

The common star pressure obtained from the left state is

and the star density on side is

In vector form, the HLLC flux is selected piecewise as

For transported species, the star-region species flux follows the HLLC mass flux and the upwind mass fraction, so conservation of total carrier mass and constituent mass remains tied to the same contact wave.