Abstract
This chapter describes the phase-field approach to modeling interface dynamics, with particular emphasis on the mathematical formulation and computational aspects. We describe to approaches to derive a phase-field model. The first one can be understood as a regularization approach: We start with a sharp interface model which is later replaced by a diffuse interface. The second approach starts with a free energy functional and balance laws for mass, linear momentum and energy; the final governing equations are derived using the second law of thermodynamics and the Coleman-Noll procedure. We finish by illustrating how the phase-field method can be used to solve problems on complicated geometries using cartesian grids only. Some of the opportunities opened by the phase-field approach are illustrated with numerical simulations.
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Notes
- 1.
The term phase may refer to different concepts. It can be used, e.g., to define the different states of matter in a solid-liquid model, the different components in a mixture, or to determine whether there is a fracture or not in a crack propagation model.
- 2.
- 3.
- 4.
Note that V n is the normal velocity of the interface, that is, V n = v LS ⋅n LS.
- 5.
The co-area formula is
$$\displaystyle \begin{aligned} \lim_{\epsilon \rightarrow 0} \frac{1}{\epsilon} \int_\Omega q\Big( \frac{d_{\Gamma_{\mathrm{int}}}(\boldsymbol{x})}{\epsilon} \Big) \,\mathrm{d} x = \alpha_q \; \int_{\Gamma_{\mathrm{int}}} \mathrm{d} a , \end{aligned} $$(41)In this case, we use a constant value for α q, where \(\alpha _q = \int _{-\infty }^\infty q(z) \,\mathrm {d} z\). The co-area formula is valid for suitably decaying functions q(z), see [21, Lemma 2.1].
- 6.
- 7.
The term constitutive class means that a certain function is allowed to depend on other variables. In this case, the constitutive class of Ψ allows it to depend on ϕ and ∇ϕ. Fundamental laws can be used to restrict even more the constitutive class of a function and allow only certain kinds of dependence. The term constitutive class is commonly employed in classical mechanics; see [37, 63].
- 8.
Mass conservation in Eq. (54), i.e., \(\frac {\mathrm {d}}{\mathrm {d} t}(\int _{\Omega }\phi \,\mathrm {d} x)=0\), is satisfied for natural boundary conditions h ⋅n a = 0 on ∂ Ω, where n a is the unit normal vector to ∂ Ω.
- 9.
The term μ h in Eq. (57) may be interpreted as an energy flux.
- 10.
Note that, on multiphase systems, balance of angular momentum does not imply the symmetry of T [7].
- 11.
If A is a symmetric tensor, then A : B = A : (B + B T)∕2. Consequently, it can easily be proven that if A is symmetric and B is skew-symmetric, then A : B = 0.
- 12.
Usually, m and ν are assumed to be constant.
- 13.
The smooth function δ Γ works as a marker of the position of the boundary of the moving domain. A suitable expression for this function could be, e.g., δ Γ = 𝜖 2|∇ϕ|2, though there are other valid expressions for δ Γ in the literature.
- 14.
Note that the velocity of ρ Γ within the surface Γρ (i.e., u Γ) does not necessarily coincide with the velocity of the surface \((\boldsymbol {u}_{\Gamma _\rho })\).
- 15.
The variational formulation corresponding to the reference problem is analogous.
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Bures, M., Moure, A., Gomez, H. (2021). Computational Treatment of Interface Dynamics via Phase-Field Modeling. In: Greiner, D., Asensio, M.I., Montenegro, R. (eds) Numerical Simulation in Physics and Engineering: Trends and Applications. SEMA SIMAI Springer Series, vol 24. Springer, Cham. https://doi.org/10.1007/978-3-030-62543-6_2
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