Starting from the findings and definitions of the previous section, the internal energy density
is presented, which is used in the following derivations of the governing differential equations. It contains bulk material and crack phase-field contributions,
\(\psi ^\text {el}\) and
\(\psi ^\text {c}\), respectively. The global incremental potential
is defined according to [
45, Equation (90)]. The index
n refers to the previous, converged time increment, whereas quantities without the index are related to the current
\((n+1)^\text {th}\) increment. The time increment is denoted by
\(\tau =t_{n+1}-t_n\). It is noted that a first order
Euler backward time integration scheme is employed for the rate
\(\dot{c}\) of the crack phase-field, which enters the dissipation potential
\(\varPhi (\dot{c})=\frac{\eta _\text {f}}{2}\dot{c}^2\). Here,
\(\eta _{\text {f}}\ge 0\) is a kinetic parameter, often referred to as viscosity, which is of purely numerical nature in this contribution. Its choice is discussed in Sect.
3. The incorporation of
\(\dot{c}\) can be understood as a viscous regularization, which makes it possible to use a monolithic solution approach. Various other approaches and their implications can be found in literature, see e.g., [
2,
46]. The vector
\(\bar{\varvec{t}}\) denotes given external tractions on
Neumann boundaries
\(\partial \varOmega _{\varvec{t}}\). The strain jump, which enters
\(\psi \), is determined within a local minimization procedure, cf. Section
2.4, and is therefore known which is indicated by the star
. Hence,
\(\varvec{u}\) and
c are obtained by the global minimization principle
$$\begin{aligned} \lbrace \varvec{u} ,c\rbrace = \arg \inf _{\varvec{u}\in {\mathcal {U}}}\inf _{c\in {\mathcal {C}}}\varPi ^\tau \end{aligned}$$
(15)
with admissible sets
$$\begin{aligned} {\mathcal {U}}(\varvec{u})&= \lbrace \varvec{u}\in \mathbb {R}^3 \;\vert \; \varvec{u} = \bar{\varvec{u}} \text {on} \partial \varOmega _{\varvec{u}}\rbrace \quad \text {and} \end{aligned}$$
(16)
$$\begin{aligned} {\mathcal {C}}(c)&= \lbrace c \in \left[ 0,1\right] \subset \mathbb {R} \;\vert \; c=0 \text {on}\varGamma ^\text {c}_0 \text {and}c({\varvec{x}})=0\text {for}c_n({\varvec{x}})<c_\text {th} \rbrace \>\text {.}\end{aligned}$$
(17)
The first constraint in
\({\mathcal {C}}\) is only relevant for the initial crack along
\(\varGamma ^\text {c}_0\). Afterwards, the second condition, also known as
fracture-like irreversibility constraint [
3,
47], suffices, where
\(c_\text {th}\ll 1\) is a small, positive threshold value. Previous investigations [
25] confirmed, that setting
\(c_\text {th}=0.03\) does not impact the crack path, while ensuring irreversibility. A discussion on different irreversibility constraints can be found in [
47]. Subsequently, the
Euler–
Lagrange equations
$$\begin{aligned} \nabla \cdot \varvec{\sigma }&={\varvec{0}}\quad \text {and} \end{aligned}$$
(18)
$$\begin{aligned} \eta _{\text {f}}\,\frac{c-c_n}{\tau }&=\frac{{\mathcal {G}}_\text {c}}{2{\ell _\text {c}}}(1-c)-2(1-\eta )\,c\,\psi ^{\text {el}}_++2{\ell _\text {c}}\nabla \cdot ({\mathcal {G}}_\text {c}\nabla c) \end{aligned}$$
(19)
can be derived, subject to
Neumann boundary conditions
$$\begin{aligned} \varvec{\sigma }^\top \cdot \varvec{n}^{\text {b}}&=\bar{\varvec{t}}\quad \text {on}\quad \partial \varOmega _{\varvec{t}}\quad \text {and} \end{aligned}$$
(20)
$$\begin{aligned} \nabla c\cdot \varvec{n}^{\text {b}}&=0\quad \text {on}\quad \partial \varOmega \>\text {,}\end{aligned}$$
(21)
where
\(\varvec{n}^{\text {b}}\) denotes the outward normal vector along the corresponding boundary. Equation (
4) has been used in Eq. (
19). The thermodynamically consistent relation for the
Cauchy stress tensor is defined by
It is noted that the chain rule has been used together with Eqs. (
10) and (
11). The next section is dedicated to the determination of the strain jump
which enters the incremental potential (
14). The validity of Eq. (
22) is demonstrated in “Appendix A”.