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Diffuse interface models in fluid mechanics

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S<strong>in</strong>ce λ is constant, s = s 0 . Therefore( ) ∂sρ T ds = ρ Cv 0 0dT + ρ T∂ρTdρThusρ Cv 0 dT( ) ∂s0dt = ∇ · (k ∇T ) − ρ T ∂ρTdρ+ τ : ∇v (55)dtThis equation is very similar to the classical equation of evolution of the temperature <strong>in</strong> as<strong>in</strong>gle-phase <strong>fluid</strong>. However, the <strong>in</strong>terpretation of the term <strong>in</strong> dρ/dt is very different. Indeed, for as<strong>in</strong>gle-phase <strong>in</strong>compressible <strong>fluid</strong>, this term vanishes (by def<strong>in</strong>ition). In the case of a liquid-vapor<strong>in</strong>terfacial zone, (dρ/dt) represents the rate of vaporization denoted γ c . Indeed, let us consideran <strong><strong>in</strong>terface</strong> where vaporization occurs. If we follow a liquid <strong>fluid</strong> particle <strong>in</strong> its motion, as itcrosses the <strong><strong>in</strong>terface</strong> to become vapor, its density drastically decreases, therefore dρ/dt < 0. Now,ρ T (∂s 0 /∂ρ) T is analogous to the latent heat (cf. (37)). Therefore, this term can be approximatedby γ c L ρ/(ρ l − ρ v ). This term is thus a spread<strong>in</strong>g of the latent heat source over the <strong>in</strong>terfacialzone.2.3 Different forms of the momentum balance equationIn the form (52) of the momemtum balance equation, the Korteweg tensor might not be the mostappropriate. Indeed, from a numerical po<strong>in</strong>t of view for <strong>in</strong>stance, the discretization of this termis not straightforward. Moreover, we will see that there exists an equivalent from <strong>in</strong> which onlyLaplacian and gradient operators appear, which is generally much easier to implement.The follow<strong>in</strong>g identity holds:∇ · (φ ⊗ ∇ρ) = ∇(ρ ∇ · φ) − ρ ∇(∇ · φ) + φ · ∇∇ρGiven the expression (45) for P and the differential of F (15), one hasThus, equation (52) readsρ dvdt∇P = ρ ∇g + ρ s ∇T − φ · ∇∇ρ= −ρ ∇ (g − ∇ · φ) − ρ s ∇T + ∇ · τThis form of the momemtum balance equation makes clearly appears the two conditions ofequilibrium (18)-(19). This shows <strong>in</strong> particular that if any of these thermodynamic equilibriumconditions is not satisfied, it triggers a <strong>fluid</strong> motion. Moreover, s<strong>in</strong>ce the thermodynamic equilibriumconditions appear <strong>in</strong> this equation, it shows its thermodynamic consistency. Moreover, froma numerical po<strong>in</strong>t of view, Jamet et al. [2002] showed that, through a detailed analysis of the discretizedenergy exchanges, this form allows to get rid of the so-called parasitic currents [Brackbillet al., 1992]. These non-physical currents, concentrated <strong>in</strong> the close vic<strong>in</strong>ity to the <strong><strong>in</strong>terface</strong>, are<strong>in</strong>duced by numerical truncation that are very difficult to elim<strong>in</strong>ate without a detailed analysisof the energy exchanges. The thermodynamic consistency of this model gives a framework todevelop accurate numerical schemes.2.4 Boundary conditions and contact angleSo far, <strong>in</strong> the determ<strong>in</strong>ation of the equilibrium conditions or of the equations of motion, we havenot studied the boundary conditions that must be applied on the density field. In this section,19

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