Abstract
The article is devoted to the asymptotic limit of the compressible Navier–Stokes system with a pressure obeying a hard–sphere equation of state on a domain expanding to the whole physical space \(\textbf{R}^3\). Under the assumptions that acoustic waves generated in the case of ill-prepared data do not reach the boundary of the expanding domain in the given time interval and a certain relation between the Reynolds and Mach numbers and the radius of the expanding domain we prove that the target system is the incompressible Euler system on \(\textbf{R}^3\). We also provide an estimate of the rate of convergence expressed in terms of characteristic numbers and the radius of domains.
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Notes
Several works are devoted to the study of macroscopic models for heterogeneous media like mixtures, suspensions or crowds, in dense regimes. These regimes show interesting behaviors such as transition phases with congestion (also called jamming for granular flows) and non-local (in time and/or in space) effects which are both due to a physical packing constraint, that is the finite size of the microscopic components. At the macroscopic scale this limitation corresponds to a maximal density constraint \( \rho \le \rho ^{*}\). A very challenging question in physics and mathematics is to model and analyze the change of behavior in congested domains \(\rho = \rho ^{*}\) and close to a transition phase \(\rho ^{*}-\epsilon<\rho <\rho ^{*}\). Two different ways are generally considered in the literature to model congestion phenomena at the macroscopic level. The first approach, called hard approach, consists in coupling compressible dynamics in the free domain \(\{\rho < \rho ^{*} \}\), with incompressible dynamics in the congested domain \(\{\rho = \rho ^{*} \}\). Associated to the incompressibility constraint on the velocity field, an additional potential (seen as the Lagrange multiplier) is activated in the congested regions. The second approach is called soft approach, prevents the apparition of congested phases by introducing in the compressible dynamics repulsive forces which become singular as \(\rho \) approaches \(\rho ^{*}\). A first generic hard congestion model is derived in [7] by Bouchut et al. from one-dimensional two-phase gas/liquid flows for more details on the model see e.g. [6, Section 2].
The system proposed by Bouchut was studied theoretically by Berthelin in [1, 12]. Degond et al. applied numerical discretization, see [11, 12], to solve the soft congestion system. Let us also mention on the subject the study [5] which addresses the issue of the creation of congested zones in 1D and highlights the multi-scale nature of the problem.
In paper [6] authors study the compressible Brinkman equations, where maximal packing is encoded in a singular pressure and a singular bulk viscosity. It was shown that the global weak solutions converge (up to a subsequence) to global weak solutions of the two-phase compressible/incompressible Brinkman equations with respect to a parameter \(\varepsilon \) which measures effects close to the maximal packing value. Depending on the importance of the bulk viscosity with respect to the pressure in the dense regimes, memory effects are activated or not at the limit in the congested (incompressible) domain. At the limit on the hard congestion system, authors cover in particular the two cases introduced in [35] and [36] where pressure effects or memory effects are activated. The first justification of the link between a soft congestion system and a hard congestion system is given in [4] for the one-dimensional case. More details concerning soft and hard congestion problem can be found in [6], Sect. 2. In the paper [3] the singular limits of Euler equations with hard-sphere pressure towards the constrained Euler equations for smooth solutions are investigated.
In fact for \(\Omega \subset \textbf{R}^2\), \(W^{1,2}(\Omega )\) is embedded into \(L^q(\Omega )\) for any \(q\in [1,\infty )\) but the better integrability will not bring any benefits in further analysis. For the sake of clarity we will not distinguish between the 2d and 3d case.
Let us mention that the incompressible inviscid limit was investigated by Lions and Masmoudi [28] in the case of well–prepared initial data. A different approach by using Strichartz’s estimates for the linear wave equation has been developed by Schochet in [39]. For the application of Strichartz’s estimates in the case of low Mach number limit the reader can consult the work of Desjardins and Grenier [10]. The incompressible inviscid limit in the case of ill-prepared initial data was studied by Masmoudi [31] on the whole space and also on the torus.
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Acknowledgements
Š. N. and M. K. have been supported by the Czech Science Foundation (GAČR) project 22-01591 S. Moreover, Š. N. and M. K. have been supported by Praemium Academiae of Š. Nečasová. The Institute of Mathematics, CAS is supported by RVO:67985840.
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Appendix
Appendix
The ensuing lemma deals with renormalized solutions of the continuity equation. It collects versions of assertions [34, Lemmas 6.9 and 6.11] adopted for a function b considered in this paper.
Lemma 4.1
Let \(T>0\) and \(\Omega \subset \textbf{R}^d\), \(d\ge 2\), be a bounded Lipschitz domain. Let \(\rho \in L^\infty (Q_T)\) be such that \(0\le \rho <{\bar{\rho }}\) a.e. in \(Q_T\) and \(\rho \) together with \(u\in L^2(W^{1,2}_0(\Omega )^d)\) satisfy the continuity equation
Let \(b\in C^1([0,{\bar{\rho }}))\) be a nonnegative function such that
and
Let \(\rho \) and u be extended by zero in \((0,T)\times \left( \textbf{R}^d\setminus \Omega \right) \).
-
1.
Then the continuity equation (107) holds in the sense of renormalized solutions
$$\begin{aligned} \partial _tb(\rho )+{\textrm{div}}(b(\rho )u)+(b'(\rho )\rho -b(\rho )){\textrm{div}}u=0\text { in }{\mathcal {D}}'((0,T)\times \textbf{R}^d), \end{aligned}$$(110) -
2.
Moreover, for \(b_\alpha \) with \(\alpha \in (0,\alpha _0)\) defined as
$$\begin{aligned} b_\alpha (s)={\left\{ \begin{array}{ll} b(s)&{}s\le {\bar{\rho }}-\alpha ,\\ b({\bar{\rho }}-\alpha )&{}s>{\bar{\rho }}-\alpha \end{array}\right. } \end{aligned}$$(111)the renormalized continuity equation holds in the form
$$\begin{aligned} \partial _tb_\alpha (\rho )+{\textrm{div}}(b_\alpha (\rho )u)+(b'_\alpha (\rho )\rho -b_\alpha (\rho )){\textrm{div}}u=0\text { in }{\mathcal {D}}'((0,T)\times \textbf{R}^d), \end{aligned}$$(112)where we set \(b'_\alpha (\rho )=0\) in \(\{\rho ={\bar{\rho }}-\alpha \}\).
Proof
Applying the extension procedure from [34, Lemma 6.8] we get
for the extensions \(\rho \in L^\infty ((0,T)\times \textbf{R}^d)\) and \(u\in L^2(0,T;W^{1,2}_{loc}(\textbf{R}^d))\) of \(\rho \) and u from assumptions of the lemma by zero in \((0,T)\times \left( \textbf{R}^d\setminus \Omega \right) \). Regularizing the latter equation over the spatial variables by the usual mollifier \(S_\varepsilon \) with \(\varepsilon >0\) yields
where
cf. [34, Lemma 6.7]. We observe that
We fix \(\delta \in (0,\alpha _0)\), extend \(b(s)=b(-s)\) on \([-\alpha _0,0]\) and define \(b_{(\delta )}(\cdot )=b(\cdot -\delta )\). Next we multiply (113) on \(b_{(\delta )}'(S_\varepsilon (\rho ))\) and obtain
The approximating property
implies the existence of a nonrelabeled subsequence \(\{S_\varepsilon (\rho )\}\) such that \(S_\varepsilon (\rho )\rightarrow \rho \) a.e. in \((0,T)\times \textbf{R}^d\). Taking into account the continuity of \(b^{(j)}\), where \(j\in \{0,1\}\) denotes the order of the derivative, we have \(b^{(j)}_{(\delta )}(S_\varepsilon (\rho ))\rightarrow b^{(j)}_{(\delta )}(\rho )\) a.e. in \((0,T)\times \textbf{R}^d\). Taking into consideration also (118120) and (109) it follows that
We note that (109) implies that \(b'\ge 0\) on \(({\bar{\rho }}-\alpha _0,{\bar{\rho }})\) so that \(|b'_{(\delta )}(S_\varepsilon (\rho ))|=b'_{(\delta )}(S_\varepsilon (\rho ))\le b'_{(\delta )}({\bar{\rho }})\) for \(S_\varepsilon (\rho )-\delta >{\bar{\rho }}-\alpha _0\). Hence we can apply the Lebesgue dominated convergence theorem to infer
for any \(p\in [1,\infty )\). The latter convergences and (117) imply
Combining (116), (114), (119) and the latter convergence one arrives at (110) for \(b=b_{(\delta )}\). Now we pass to the limit \(\delta \rightarrow 0_+\). We have \(b^{(j)}_{(\delta )}(\rho )\rightarrow b^{(j)}(\rho )\) a.e. in \((0,T)\times \textbf{R}^d\), \(j\in \{0,1\}\). Moreover, (109) implies
Hence we infer by the Lebesgue dominated convergence theorem and (108)
Having the latter convergences at hand we pass to the limit \(\delta \rightarrow 0_+\) in (110) with \(b=b_{(\delta )}\) and the first assertion of the lemma is proved.
In order to prove the second assertion, we begin with the proof of the following auxiliary identity
To this end we consider \(b\in C^1_c((0,\infty ))\) such that \(b(s)=s\) in \([\tfrac{3}{4}({\bar{\rho }}-\alpha ),{\bar{\rho }}-\tfrac{3}{4}\alpha ]\) and b, \(b'\) are nondecreasing in \([{\bar{\rho }}-\tfrac{\alpha }{2},{\bar{\rho }}]\). We define \(b^+_{\alpha ,\varepsilon }=S_\frac{\varepsilon }{2}(b_{\alpha +\varepsilon })\), \(b^-_{\alpha ,\varepsilon }=S_\frac{\varepsilon }{2}(b_{\alpha -\varepsilon })\). Then we have as \(\varepsilon \rightarrow 0_+\)
By the first assertion of the lemma we have
Letting \(\varepsilon \rightarrow 0_+\) and employing the convergences from (122) we deduce by the Lebesgue dominated convergence theorem from the latter identities
Subtracting the latter equations we conclude (121).
Next, we consider for fixed \(\varepsilon <\alpha \) \(S_\varepsilon (b_\alpha )\), the mollification of \(b_\alpha \) extended by \(b({\bar{\rho }}-\alpha )\) in \(({\bar{\rho }},{\bar{\rho }}+1]\) and by 0 outside of \([0,{\bar{\rho }}+1]\). As \(S_\varepsilon (b_\alpha )\) is constant in a vicinity of \({\overline{\rho }}\), it fulfills (109) and \(S_\varepsilon (b_\alpha )(\rho )\) satisfies (19), it follows that
Furthermore, we have as \(\varepsilon \rightarrow 0_+\)
Hence we infer that as \(\varepsilon \rightarrow 0_+\)
Employing (121) we deduce that \(\rho (S_\varepsilon (b_\alpha ))'(\rho ){\textrm{div}}u=0\) a.e. in \(\{\rho ={\bar{\rho }}-\alpha \}\). Using the convergences from (124), the uniform bounds with respect to \(\varepsilon \) on \(S_\varepsilon (b_\alpha ), S_\varepsilon (b_\alpha )'\) and the Lebesgue dominated convergence theorem we pass to the limit \(\varepsilon \rightarrow 0_+\) in (123) to conclude (112). \(\square \)
Lemma 4.2
Let \(\Omega \subset \textbf{R}^d\) be a starshaped domain with respect to a ball B possessing the radius R. There exists a linear operator \({\mathcal {B}}: C_c^\infty (\Omega )\rightarrow C_c^\infty (\Omega )^d\) such that \({\textrm{div}}{\mathcal {B}}(f)=f\) provided that \(\int _\Omega f=0\). Moreover, \({\mathcal {B}}\) can be extended in a unique way as a bounded linear operator
-
1.
\({\mathcal {B}}: L^p(\Omega )\rightarrow W^{1,p}(\Omega )^d\) such that \(\Vert B(f)\Vert _{W^{1,p}(\Omega )}\le c\Vert f\Vert _{L^p(\Omega )}\)
-
2.
\({\mathcal {B}}: \{f\in (W^{1,p'}(\Omega ))':\langle f,1\rangle =0\}\rightarrow L^p(\Omega )^d\) such that \(\Vert B(f)\Vert _{L^p(\Omega )}\le c\Vert f\Vert _{(W^{1,p}(\Omega ))'}\)
for any \(p\in (1,\infty )\) where the constants c take the form
Assertions in the following lemma are based on the results from [23]
Lemma 4.3
Let \(v_0\in W^{m,2}(\textbf{R}^3)\) with \(m>4\) be such that \({\textrm{div}}v_0=0\) in \(\textbf{R}^3\). Then there is \(T_{max}>0\) and a classical solution v, unique in the class
to the initial value problem
Furthermore, the associate pressure \(\Pi \) can be expressed as
implying particularly that \(\Pi \in C^1([0,T];C^1(\textbf{R}^3)\cap W^{1,2}(\textbf{R}^3))\), \(T\in (0,T_{max})\).
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Kalousek, M., Nečasová, Š. Singular Limit for the Compressible Navier–Stokes Equations with the Hard Sphere Pressure Law on Expanding Domains. J. Math. Fluid Mech. 25, 17 (2023). https://doi.org/10.1007/s00021-022-00750-y
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DOI: https://doi.org/10.1007/s00021-022-00750-y
Keywords
- Compressible Navier–Stokes equations
- Hard–sphere pressure
- Expanding domain
- Low Mach number limit
- Vanishing viscosity limit