Incompressibility is a common assumption made of the mechanical properties of many materials. This is, of course, an approximation as many materials relevant to the tissue engineering community have a large bulk modulus in reality, but are not absolutely incompressible [
37,
38]. In this section, we explore how the model developed in Sect.
2 can be adapted to account for an incompressible component in the composite material. Primarily, this involves a different formulation of the microscale mechanical model, due to the differing constitutive equations on the microscale. Without loss of generality we have chosen to set the inner material A to be incompressible, noting that the analysis would follow similarly if the outer material B was chosen to be incompressible instead.
The analysis follows that of the SAH model given in Sect.
2, except that in material A, instead of using (
1), (
2), we use the incompressible linearly elastic Navier equations, which are given by
$$\begin{aligned}&-\frac{\partial p^*}{\partial X_k^*}+\mu _A\left( \frac{\partial ^2 u_k^{A*}}{\partial X_i^* \partial X_i^*}+\frac{\partial ^2 u_k^{A*}}{\partial {z^*}^2}\right) =0, \end{aligned}$$
(48)
$$\begin{aligned}&-\frac{\partial p^*}{\partial z^*}+\mu _A\left( \frac{\partial ^2 w^{A*}}{\partial X_i^* \partial X_i^*}+\frac{\partial ^2 w^{A*}}{\partial {z^*}^2}\right) =0, \end{aligned}$$
(49)
and
$$\begin{aligned} \frac{\partial u_k^{A*}}{\partial X_k^*}+\frac{\partial w^{A*}}{\partial z^*}=0, \end{aligned}$$
(50)
where
\(p^*\) is the non-dimensional pressure in A. The same non-dimensionalise scalings (
6) as in Sect.
2 are adopted, but with the addition of the unknown isotropic unknown pressure which is scaled
\(p^*=Pp+p_0\) where
\(p_0\) is atmospheric pressure.
Note, as in the compressible–compressible case, the stress tensor scaling
\(\tau _{ij}^{B*}=\mu _B \epsilon ^{-1} \tau _{ij}^B\) is used and therefore, to ensure continuity of stress on the interface
\(\Gamma \) between the two materials, we must take
\(\tau _{ij}^{A*} = \mu _A \epsilon ^{-1} \tau _{ij}^A\). Moreover, assuming that the pressure in the incompressible material can potentially contribute to the leading-order effective composite stress, the scaling
\(P=\mu _A \epsilon ^{-1}\) is assumed. As before
\(\epsilon =\frac{\delta }{d}\),
\(\mu =\frac{\mu _A}{\mu _B}\) and
\(\alpha _B=\frac{\lambda _B}{\mu _B}\). As in the general case, we assume
\(\mu \),
\(\alpha _{A, B}\) and
\(\beta _{A, B}\) to be of order unity and the non-dimensional equations in
\(\Omega _A\) are now
$$\begin{aligned}&-\frac{\partial p}{\partial X_k}+\frac{\partial ^2 u_k^A}{\partial X_i \partial X_i}+\epsilon ^2 \frac{\partial ^2 u_k^A}{\partial z^2}=0, \end{aligned}$$
(51)
$$\begin{aligned}&-\epsilon \frac{\partial p}{\partial z}+\frac{\partial ^2 w^A}{\partial X_i \partial X_i}+\epsilon ^2 \frac{\partial ^2 w^A}{\partial z^2}=0, \end{aligned}$$
(52)
and
$$\begin{aligned} \frac{\partial u_k^A}{\partial X_k}+\epsilon \frac{\partial w^A}{\partial z}=0. \end{aligned}$$
(53)
In
\(\Omega _B\) the non-dimensional equations are
$$\begin{aligned} (1+\alpha _B) \left( \frac{\partial ^2 u_i^B}{\partial X_k \partial X_i}+\epsilon \frac{\partial ^2 w^B}{\partial X_k \partial z} \right) +\frac{\partial ^2 u_k^B}{\partial X_i \partial X_i}+\epsilon ^2 \frac{\partial ^2 u_k^B}{\partial z^2}=0, \end{aligned}$$
(54)
and
$$\begin{aligned} (1+\alpha _B)\left( \epsilon \frac{\partial ^2 u_i^B}{\partial z \partial X_i}+\epsilon ^2 \frac{\partial ^2 w^B}{\partial z^2}\right) +\frac{\partial ^2 w^B}{\partial X_i \partial X_i}+\epsilon ^2 \frac{\partial ^2 w^B}{\partial z^2}=0. \end{aligned}$$
(55)
The same usual conditions of continuity of displacement and stress, (
9), are applied at the interface
\(\Gamma \) between the two materials, but note that now
$$\begin{aligned} \tau _{ij}^A = -p\delta _{ij} +\frac{\partial u_i^A}{\partial X_j}+\frac{\partial u_j^A}{\partial X_i} \quad \text {and}\quad \tau _{i3}^A = \frac{\partial w^A}{\partial X_i}+\epsilon \frac{\partial u_i^A}{\partial z}. \end{aligned}$$
(56)
As utilised in Sect.
2, we introduce the macroscale coefficient
\(x_k=\epsilon X_k\) and equate coefficients of
\(\epsilon ^0\) in equations (
51)–(
55) and in the boundary conditions (
9) on
\(\Gamma \). Then leading-order solution is identical to the general case as expected with the addition requirement that
\(p^{(0)}=p^{(0)}({\mathbf {x}}, z).\) The continuity of stress boundary condition reduces this to
\(p^{(0)}=0\) on
\(\Gamma \) and, hence, we require
\(p^{(0)}=0\) for all
\({\mathbf {x}}\) and
z. Leading-order variations in incompressible pressure, therefore, only occur on the microscale.
3.1 Microscale problem
By equating coefficients of
\(\epsilon ^1\) in Eqs. (
51)–(
55) and boundary conditions (
9), we obtain the counterparts of Eqs. (
15) for material B (with incompressible version for A) that define the microscale cell problem. The same ansatzes, (
19), (
20), as the general case applies, but an additional expression of the form
$$\begin{aligned} p^{(1)}=P^1({\mathbf {X}}) \frac{\partial u^{(0)}}{\partial x}+P^2({\mathbf {X}}) \frac{\partial v^{(0)}}{\partial y} +Q({\mathbf {X}}) \frac{\partial w^{(0)}}{\partial z} \end{aligned}$$
(57)
is included to account for the isotropic pressure term in material A. These ansatzes allow us to consider coefficients of macroscale derivatives and so formulate the cell problem solely in terms of the microscale. This microscale cell problem again conveniently uncouples into three systems as in (
21)–(
29) that may be stated separately as follows:
For
\(W_{\Omega i}^{pq}\):
$$\begin{aligned}&\frac{\partial ^2 W_{Ak}^{pq}}{\partial X_i \partial X_i}={\left\{ \begin{array}{ll} \frac{\partial P^p}{\partial X_k} \quad \text {when} \quad p=q, \\ 0 \quad \text {otherwise} \end{array}\right. } \quad \text {and} \quad \frac{\partial W_{Ak}^{pq}}{\partial X_k}+\delta _{pq}=0 \quad \text {on }\Omega _A, \end{aligned}$$
(58)
$$\begin{aligned}&(1+\alpha _B) \frac{\partial ^2 W_{Bi}^{pq}}{\partial X_k \partial X_i}+\frac{\partial ^2 W_{Bk}^{pq}}{\partial X_i \partial X_i}=0 \quad \text {on }\Omega _B, \end{aligned}$$
(59)
with boundary conditions on
\(\Gamma \) that
\(W_{Ak}^{pq}=W_{Bk}^{pq}\), as before, and
$$\begin{aligned}&\alpha _B n_j \left( \frac{\partial W_{Bk}^{pq}}{\partial X_k}+\delta _{pq}\right) + n_i \left( \frac{\partial W_{Bi}^{pq}}{\partial X_j}+\frac{\partial W_{Bj}^{pq}}{\partial X_i}\right) + n_i (\delta _{ip} \delta _{jq}+\delta _{jp} \delta _{iq}) \nonumber \\&\quad = n_i \mu \left( \frac{\partial W_{Ai}^{pq}}{\partial X_j}+\frac{\partial W_{Aj}^{pq}}{\partial X_i}\right) +n_i \mu ( \delta _{ip} \delta _{jq}+\delta _{jp} \delta _{iq})+ {\left\{ \begin{array}{ll} -P^p \mu n_j \quad \text {when} \quad p=q, \\ 0 \quad \text {otherwise}. \end{array}\right. } \end{aligned}$$
(60)
For
\(W_{\Omega i}^{0}\):
$$\begin{aligned}&\frac{\partial ^2 W_{Ak}^0}{\partial X_i \partial X_i}=\frac{\partial Q}{\partial X_k} \quad \text {and} \quad \frac{\partial W_{Ak}^0}{\partial X_k}+1=0 \quad \text {on }\Omega _A, \end{aligned}$$
(61)
$$\begin{aligned}&(1+\alpha _B) \frac{\partial ^2 W_{Bi}^0}{\partial X_k \partial X_i}+\frac{\partial ^2 W_{Bk}^0}{\partial X_i \partial X_i}=0 \quad \text {on }\Omega _B, \end{aligned}$$
(62)
with boundary conditions on
\(\Gamma \) that
\(W_{Ai}^0=W_{Bi}^0\) as before and
$$\begin{aligned} \alpha _B n_j \left( \frac{\partial W_{Bk}^0}{\partial X_k}+1\right) + n_i \left( \frac{\partial W_{Bi}^0}{\partial X_j}+\frac{\partial W_{Bj}^0}{\partial X_i}\right) =-n_j \mu Q +n_i\mu \left( \frac{\partial W_{Ai}^0}{\partial X_j}+\frac{\partial W_{Aj}^0}{\partial X_i}\right) . \end{aligned}$$
(63)
For
\(\phi _\Omega ^p\):
this system of
\(\phi _\Omega ^p\) is identical to Eqs. (
27)–(
29) in the general case.
3.2 Deriving the effective macroscale equations
By equating coefficients of
\(\epsilon ^1\) in Eqs. (
51)–(
55) and boundary conditions (
9), and following the same process as in Sect.
2.3 the second-order governing equations are obtained for the compressible–incompressible setup. These equations are further reduced using the coefficients of
\(\epsilon \) in the continuity equation (
53) to obtain
$$\begin{aligned} \frac{\partial \tau _{ik}^{A(2)}}{\partial X_i}&+\frac{\partial ^2 u_{i}^{A(1)}}{\partial X_k \partial X_i}+\frac{\partial ^2 w^{A(1)}}{\partial X_k \partial z}+\frac{\partial ^2 u_i^{(0)}}{\partial x_k \partial x_i}+\frac{\partial ^2 w^{(0)}}{\partial x_k \partial z}-\frac{\partial p^{(1)}}{\partial x_k} \nonumber \\&+\frac{\partial ^2 u_{k}^{A(1)}}{\partial x_i \partial X_i}+\frac{\partial ^2 u_k^{(0)}}{\partial x_i \partial x_i}+\frac{\partial ^2 u_k^{(0)}}{\partial z^2}=0, \end{aligned}$$
(64)
and
$$\begin{aligned} \frac{\partial \tau _{i3}^{A(2)}}{\partial X_i}-\frac{\partial p^{(1)}}{\partial z}+\frac{\partial ^2 w^{A(1)}}{\partial X_i \partial x_i}+\frac{\partial ^2 w^{(0)}}{\partial x_i \partial x_i}+\frac{\partial ^2 u_i^{(0)}}{\partial z \partial z_i}+2\frac{\partial ^2 w^{(0)}}{\partial z^2}=0. \end{aligned}$$
(65)
By integrating over the cell, adding the equations in the two materials, and then using the continuity of stress boundary condition and the Divergence Theorem, we are able to eliminate terms involving second-order variables. From this, we obtain the same homogenised equations (
37), (
38) as derived in the general case, with the same microscale averaged parameters
\(K_{pqki}\),
\(K_{ik}^0\),
\(H_{pk}\) and
\(A_2\), given by (
39)–(
41), (
44), (
45). The incompressibility of material A, however, causes
\( G_{pq}\),
\( G^0\) and
\(A_1\) to be redefined in terms of the isotropic pressure terms of the ansatz as follows:
$$\begin{aligned} G_{pq}= & {} \alpha _B \iint _{\Omega _B} \, \frac{\partial W_{Bi}^{pq}}{\partial X_i} \, \mathrm {d}A- \mu {\left\{ \begin{array}{ll} \iint _{\Omega _A} \, P^p \, \mathrm {d}A \quad \text {when} \quad p=q, \\ 0 \quad \text {otherwise}, \end{array}\right. } \end{aligned}$$
(66)
$$\begin{aligned} G^0= & {} \alpha _B \iint _{\Omega _B} \, \frac{\partial W_{Bi}^0}{\partial X_i} \, \mathrm {d}A- \mu \iint _{\Omega _A} \, Q \, \mathrm {d}A, \end{aligned}$$
(67)
and
$$\begin{aligned} A_1 = \mu |\Omega _A|+(1+\alpha _B) |\Omega _B|. \end{aligned}$$
(68)
3.3 Implementation of the compressible–incompressible model
As the homogenised equations in Sects.
2 and
3 are unchanged, we may use the same macroscale elastic tensors as those given in Appendix
B. The setup of the microscale to evaluate the averaged microscale parameters requires modification as described below.
Solving the microscale system of equations, (
27)–(
29), for
\(\phi _\Omega ^p\) is trivial to input into COMSOL Multiphysics as described in Sect.
2. Due to the presence of the constraints from the continuity equation, however, the implementation of the other systems is more complex. For solving Eqs. (
58)–(
60) with
\(p = q\) and Eqs. (
61)–(
63), it is helpful to introduce a potential function
\(\psi ^i\) for
\(i=1, 2\) or 3 such that
$$\begin{aligned} W_{A1}^0&= \frac{\partial \psi ^3}{\partial X},\quad W_{A2}^0 = \frac{\partial \psi ^3}{\partial Y}, \end{aligned}$$
(69)
$$\begin{aligned} W_{A1}^{11}&= \frac{\partial \psi ^1}{\partial X},\quad W_{A2}^{11} = \frac{\partial \psi ^1}{\partial Y}, \end{aligned}$$
(70)
$$\begin{aligned} W_{A1}^{22}&= \frac{\partial \psi ^2}{\partial X},\quad W_{A2}^{22} = \frac{\partial \psi ^2}{\partial Y}. \end{aligned}$$
(71)
Without loss of generality, we set that
$$\begin{aligned} Q= \frac{\partial ^2 \psi ^3}{\partial X_i \partial X_i} \quad \text {and} \quad P^i = \frac{\partial ^2 \psi ^i}{\partial X_j \partial X_j}, \end{aligned}$$
(72)
for
\(i=1, 2\), to ensure that the only equation we need to solve for each
\(\psi ^i\) will be the constraints resulting from the continuity equations in each case.
On the other hand, for Eqs. (
58)–(
60) where
\(p\ne q\) we introduce a streamfunction
\(\zeta \) such that
$$\begin{aligned} W_{A1}^{12} = \frac{\partial \xi ^1}{\partial Y}, \quad W_{A2}^{12} = -\frac{\partial \xi ^1}{\partial X}, \quad W_{A1}^{21} = \frac{\partial \xi ^2}{\partial Y}, \quad \text {and}\quad W_{A2}^{21} = -\frac{\partial \xi ^2}{\partial X}, \end{aligned}$$
(73)
that satisfies the constraints resulting from the continuity equation and leaves us with the two remaining governing equations to solve for
\(\xi \) and the pressure variable in each case.