Abstract
We consider the evolutionary compressible Navier–Stokes equations in a two-dimensional perforated domain, and show that in the subcritical case of very tiny holes, the density and velocity converge to a solution of the evolutionary compressible Navier–Stokes equations in the non-perforated domain.
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Acknowledgements
Š. N. and F. O. have been supported by the Czech Science Foundation (GAČR) Project 22-01591 S. Moreover, Š. N. has been supported by Praemium Academiæ of Š. Nečasová. The Institute of Mathematics, CAS is supported by RVO:67985840.
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Appendix A: Bogovskiĭ’s operator in 2D and improved pressure estimates
Appendix A: Bogovskiĭ’s operator in 2D and improved pressure estimates
In this section, we give an inverse to the divergence in the two-dimensional perforated domain, and estimate its norm in any \(L^q(D_\varepsilon )\). To the best of the authors’ knowledge, such estimates for two spatial dimensions are just known in the \(L^2\)-setting, see [24, Section 1.4]. Therefore, we give here an explicit proof, which might be of independent interest. As an application, we explain how to use it to prove Lemma 3.2.
Theorem A.1
Let \(D\subset {\mathbb {R}}^2\) be a bounded domain with smooth boundary and \(D_\varepsilon \) be defined as in (3). Then, there exists an operator \({\mathcal {B}}_\varepsilon \) such that for any \(q\ge 1\),
and for any \(f\in L_0^q(D_\varepsilon )\) we have
where
and \(\varpi _\varepsilon \) is as in (19).
Proof
We follow the idea of [9], where \(L^q\)-estimates are given for the case of three spatial dimensions. Let \(f\in L_0^q(D_\varepsilon )\). Then, there exists a function \({\textbf{u}}\in W_0^{1,q}(D)\) such that
for some constant \(C>0\) independent of \(\varepsilon \) (see [5, 13]). However, \({\textbf{u}}\) does not vanish on the holes in general. To overcome this, note that the domains \(B_{\varpi _\varepsilon a_\varepsilon }(z_i^\varepsilon )\setminus B_{a_\varepsilon }(z_i^\varepsilon )\) are uniform John domains (see, e.g., [27, Example 3.2.2]), so for each \(i\in K_\varepsilon \), there exists a Bogovskiĭ operator \({\mathcal {B}}_{i,\varepsilon }\) satisfying
for some constant \(C>0\) independent of \(\varepsilon \) (see [8, Theorem 5.2]). Furthermore, we define \(\mathfrak {y}_\varepsilon \) as in (12), and
As before, set for \(z_i^\varepsilon \in K_\varepsilon \) and \(x\in D\) the functions \(\eta _\varepsilon ^i(x)=\mathfrak {y}_\varepsilon (|x-z_i^\varepsilon |)\) and \(\theta _\varepsilon ^i(x)=\vartheta _\varepsilon (|x-z_i^\varepsilon |)\), and define for \({\textbf{u}}\in W^{1,q}(B_{\varpi _\varepsilon a_\varepsilon }(z_i^\varepsilon ))\) the operator \(L_{i,\varepsilon }\) as
Note that this immediately implies \(L_{i,\varepsilon }{\textbf{u}}=0\) on \(\partial B_{\varpi _\varepsilon a_\varepsilon }(z_i^\varepsilon )\) as well as \(L_{i,\varepsilon }{\textbf{u}}={\textbf{u}}\) on \(\partial B_{a_\varepsilon }(z_i^\varepsilon )\). Moreover, by Poincaré’s inequality,
for some constant \(C>0\) independent of \(\varepsilon \). Hence, by the estimate (13) and Hölder’s inequality,
yielding an operator \(L_{i,\varepsilon }:W^{1,q}(B_{\varpi _\varepsilon a_\varepsilon }(z_i^\varepsilon ))\rightarrow W_0^{1,q}(B_{\varpi _\varepsilon a_\varepsilon }(z_i^\varepsilon ))\). Eventually, we define
Note that this operator is well defined due to
since \(L_{i,\varepsilon }{\textbf{u}}=0\) on \(\partial B_{\varpi _\varepsilon a_\varepsilon }(z_i^\varepsilon )\). Furthermore, for any \(x\in B_{a_\varepsilon }(z_i^\varepsilon )\),
by \(L_{i,\varepsilon }{\textbf{u}}={\textbf{u}}\) in \(B_{a_\varepsilon }(z_i^\varepsilon )\) and \(\tilde{f}(x)=0\) on \(D\setminus D_\varepsilon \). Hence,
as wished. Moreover, this leads for any \(x\in B_{a_\varepsilon }(z_i^\varepsilon )\) to
so indeed \({\mathcal {B}}_\varepsilon (f)=0\) on \(D\setminus D_\varepsilon \). Seeing finally that the holes \(B_{\varpi _\varepsilon a_\varepsilon }(z_i^\varepsilon )\) are disjoint, we sum up the estimates obtained to finish the proof of the theorem. \(\square \)
With the help of the operator \({\mathcal {B}}_\varepsilon \), we can show Lemma 3.2. Recalling \(a_\varepsilon =\exp (-\varepsilon ^{-\alpha })\) for some \(\alpha >2\) and \(\varpi _\varepsilon = \varepsilon ^{1+\delta }a_\varepsilon ^{-1}\) from (19), we have for any \(1\le q<2\) the bound
which is uniform as long as \(\delta \le \alpha -1\). Similarly, for \(q=2\), we have
as long as \(\delta \le \frac{\alpha -2}{2}\). The idea is now to test the momentum equation (7) by the function
for \(\theta <\gamma -1\) and some \(\xi \in C_c^\infty ([0,T))\). Note that the function \(\varphi \) is not regular enough in the time variable to use it as test function, however, one can overcome this by using a time-regularization argument (see [10, Section 2.2.5] for details). The proof of the improved integrability of the density now follows the same lines as [6, Appendix B] (see also [27, Section 4.2.2]).
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Nečasová, Š., Oschmann, F. Homogenization of the two-dimensional evolutionary compressible Navier–Stokes equations. Calc. Var. 62, 184 (2023). https://doi.org/10.1007/s00526-023-02526-2
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DOI: https://doi.org/10.1007/s00526-023-02526-2