Theory for the Phase Field in Solids Interface
The Phase Field in Solids interface solves an Allen–Cahn-type of a reaction-diffusion equation. This equation is commonly used for regularized modeling of the evolution of sharp interfaces such as cracks, damage, and grain boundaries in solids. The equation is based on the phase-field theory of fracture presented in Ref. 172. The central idea relies on approximating the set Γ that represents sharp interfaces by a regularized crack functional
(3-280)
Here, the so-called crack surface density function γ(ϕ, ∇ϕ) is a function of the phase field ϕ and its gradient ∇ϕ, which is defined in the whole domain Ω instead of only on the crack surfaces. The crack surface density function γ also depends on the internal length scale lint that controls the regularization, which means that Γl → Γ for lint → 0.
The evolution of the functional is written (Ref. 173)
(3-281)
where Sl is a driving source term, Rl is a viscous resistance term, and the inequality indicates the irreversibility of processes like damage and fracture. For a general crack surface density function with source and viscous resistance terms of the form
(3-282) and
the local form of Equation 3-281 can be derived as
(3-283)
Herein, τ is a viscous regularization time constant and f is a local source term. In the derivation, homogeneous Neumann conditions are assumed on the exterior boundaries of the domain, that is,
(3-284)
where N is the normal to the undeformed surface.
A common form for the crack surface density function is isotropic and quadratic in the phase field and its gradient (for example, Refs. 172174), which is often referred to as the AT2 (Ambrosio–Tortorelli type 2) model. The crack surface density function reads
(3-285)
By inserting Equation 3-285 into Equation 3-283, the strong form of the phase field equation reads
(3-286)
The weak form of Equation 3-286 is the default equation solved in the Phase Field in Solids interface.
Alternative phase field models of fracture have considered a crack surface density function that deviate from the local quadratic term ϕ2 and/or include anisotropy in the form of a structure tensor D in the nonlocal term (see Ref. 174 for a review). In the Phase Field in Solids interface, both the AT1 model
and the PF–CZM (phase-field regularized cohesive zone model)
are available in addition to the standard AT2 formulation.
It is also possible to specify the phase field equation based on a generalization of Equation 3-286, which also includes an extension to multiple phase fields ϕk:
(3-287)
Here, the potential function Q1, ϕ2, , ϕn) has been introduced. Equation 3-286 is recovered for the quadratic potential
(3-288)
and the structure tensor Dk = I, which corresponds to the so-called AT2 phase-field model. Note that, in absence of a source term f, the quadratic form of the AT2 model has the advantage of admitting the trivial solution ϕ = 0 as well as guaranteeing that the solution is bounded, ϕ ∈ [0, 1] (Ref. 172). If required, bounds on the phase field variable can be added in terms of weak inequality constraints; see Bounds in The Phase Field in Solids Interface.