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Global classical solutions to the viscous two-phase flow model with slip boundary conditions in 3D exterior domains
Boundary Value Problems volume 2023, Article number: 46 (2023)
Abstract
We consider the two-phase flow model in 3D exterior domains with slip boundary conditions. We establish the global existence of classical solutions of this system, provided that the initial energy is suitably small. Furthermore, we prove that the pressure has large oscillations and contains vacuum states when the initial pressure allows large oscillations and a vacuum. Finally, we also obtain the large-time behavior of the classical solutions.
1 Introduction
The two-fluid flow models widely used in the petroleum industry to describe the production and transport of oil and gas through long pipelines or wells can be written as (see [19–21, 34, 42])
where \((x,t)\in \Omega \times (0, T]\), Ω is a domain in \(\mathbb{R}^{3}\). \(\rho \ge 0\), \(m\ge 0\), \(u=(u_{1},u_{2},u_{3})\), and \(P(\rho ,m)=\rho ^{\gamma}+m^{\alpha}\) (\(\gamma >1\), \(\alpha \ge 1\)) are the unknown two-phase flow model’s fluid density, velocity, and pressure, respectively. The constants μ and λ are the shear viscosity and bulk coefficients, respectively, satisfying the following physical restrictions:
In this paper, the domain Ω is the exterior of a simply connected bounded domain D in \(\mathbb{R}^{3}\), and its boundary ∂Ω is smooth. In addition, the system is studied subject to the given initial data
and the slip boundary condition
with the far field behavior
where \(n=(n^{1},n^{2},n^{3})\) is the unit outward normal vector to the boundary ∂Ω pointing outside Ω, \(\rho _{\infty}\) and \(m_{\infty}\) are the nonnegative constants.
The first condition in (1.4) is the non-penetration boundary condition, while the second one is also known in the form
where \(D(u)=(\nabla u+(\nabla u)^{\mathrm{tr}})/2\) is the deformation tensor, \(\kappa _{\tau}\) is the corresponding normal curvature of ∂Ω in the τ direction, and the symbol \(u_{\tau}\) represents the projection of tangent plane of the vector u on ∂Ω. This type of boundary condition was originally introduced by Navier [27] in 1823, which was followed by many applications, numerical studies, and analyses for various fluid mechanical problems, see, for instance, [8, 21, 31] and the references therein.
Many models are related to the two-phase model (1.1), especially the case of \(\alpha =1\) corresponds to the hydrodynamic equations, which was derived as the asymptotic limit of Vlasov–Fokker–Planck equations coupled with compressible Navier–Stokes equations, see [7, 26]. The case of \(\alpha =2\) is associated with a compressible Oldroyd-B type model with stress diffusion, see [2]. Furthermore, if we let \(m\equiv 0\), then the viscous liquid-gas two-flow model (1.1) reduces to the classical isentropic compressible Navier–Stokes equations. Compared with the isentropic compressible Navier–Stokes equations, the main difference is that the pressure law \(P(\rho ,m)=\rho ^{\gamma}+m^{\alpha}\) depends on two different variables from the continuity equations.
Before stating our main result, we briefly recall some previous known results on the viscous two-fluid model. For the one-dimensional case, Evje and Karlsen [10] obtained the first global existence result on weak solutions with large initial data subject to the domination conditions. Later, the domination condition was removed by Evje–Wen–Zhu [11] using the decomposition of the pressure term, which allows transition to each single-phase flow. Recently, Gao–Guo–Li [13] considered the Cauchy problem of the 1D viscous two-fluid model and established the global existence of strong solutions with a large initial value and vacuum. For more related results, please refer to [9, 10, 37, 38] and the references therein. For the multi-dimensional case, Yao–Zhang–Zhu [36] proved the global existence of weak solutions to the 2D Cauchy problem case when the initial energy is small and both of the initial densities are positive. Hao and Li [15] obtained the existence and uniqueness of the global strong solutions to the Cauchy problem in \(\mathbb{R}^{d}\) with \(d\geq 2\) in the framework of Besov spaces, where the possible vacuum state is included in the equilibrium state for the gas component at far field. Zhang and Zhu [40] considered the 3D Cauchy problem and proved the global existence of a strong solution when \(H^{2}\)-norm of the initial perturbation around a constant state is sufficiently small. When both phases contain a vacuum initially, Guo–Yang–Yao [14] proved the global existence of strong solutions to the 3D Cauchy problem under the assumption that initial energy is sufficiently small. Very recently, the domination condition was removed by Yu [39] for the global existence of the strong solution to the 3D case when the initial energy is small. For large initial data cases, Vasseur–Wen–Yu [32] obtained the global existence of weak solutions to the Dirichlet boundary value problem of (1.1) in \(\mathbb{R}^{3}\) with the pressure \(P(\rho ,m)=\rho ^{r}+m^{\alpha}\) (\(r>1\), \(\alpha \ge 1\)) and the domination conditions. Novotný and Pokorný [29] extended the domination condition to the case that both γ and α can touch \(\frac{9}{5}\), where more general pressure laws covering the cases of \(P(\rho ,m)=\rho ^{r}+m^{\alpha}\) (\(r>1\), \(\alpha \ge 1\)) were considered. Wen [35] obtained the global existence of weak solutions to 3D Dirichlet problem of compressible two-fluid model without any domination conditions. However, there are few results about classical solutions to compressible two-fluid model for general bounded domains, which is one of our main motivations of the present paper.
When we take \(m=0\) in (1.1), the two-phase flow model (1.1) changes into the compressible Navier–Stokes equations. In the last several decades, significant progress on the compressible Navier–Stokes equations has been achieved by many authors in the analysis of the well-posedness and large-time behavior. We only briefly review some results related to the existence of strong or classical solutions. The global classical solutions were first obtained by Matsumura–Nishida [25] for initial data close to a nonvacuum equilibrium in \(H^{3} (\mathbb{R}^{3})\). It is worth mentioning that their results have been improved by Huang–Li–Xin [18] and Li–Xin [23], in which the global existence of classical solutions is obtained with smooth initial data that are of small energy but possibly large oscillations. Very recently, for the 3D bounded domain (or 3D Exterior Domains) with slip boundary conditions, Cai–Li [5] (or Cai–Li–Lv [6]) proved the existence and large-time behavior of global classical solutions to the compressible Navier–Stokes equations. And Cai–Huang–Shi [4] proved the global existence and exponential growth of classical solutions subject to large potential forces with slip boundary condition in 3D bounded domains. For 3D bounded Domains with Non-Slip Boundary Conditions, Fan–Li [12] proved global classical solutions to the compressible Navier–Stokes system with a vacuum.
Before stating the main results, we introduce some notations and conventions used in this paper. We denote
For integer k and \(1\le q <+\infty \), the standard homogeneous Sobolev spaces are denoted as follows:
We also denote
with the norm \(\|u\|_{W^{k,q}(\Omega )}\triangleq (\sum_{|m|\le k}\|\nabla ^{m}u \|_{L^{q}(\Omega )}^{q} )^{\frac{1}{q}}\).
Simply, \(L^{q}(\Omega )\), \(D^{k,q}(\Omega )\), \(D^{k}(\Omega )\), \(W^{k,q}(\Omega )\), and \(H^{k}(\Omega )\) can be denoted by \(L^{q}\), \(D^{k,q}\), \(D^{k}\), \(W^{k,q}\) and \(H^{k}\), respectively and set that
For two \(3\times 3\) matrices \(A= \{a_{ij} \}\), \(B= \{b_{ij} \}\), the symbol \(A:B\) represents the trace of AB,
Define the initial total energy of (1.1) by:
with
Finally, for \(v=(v^{1},v^{2},v^{3})\), we set \(\nabla _{j}v=(\partial _{j}v^{1},\partial _{j}v^{2},\partial _{j}v^{3})\), for \(j=1,2,3\), \(P_{0}=P(\rho _{0},m_{0})\), and \(P_{\infty}=P(\rho _{\infty},m_{\infty})\).
Our first result is stated below:
Theorem 1.1
Let Ω be the exterior of a simply connected bounded domain in \(\mathbb{R}^{3}\) with smooth boundary ∂Ω. For \(M\ge 1\), \(\bar{\rho}\ge \rho _{\infty}+1\), \(\bar{m}\ge m_{\infty}+1\) and some \(q\in (3,6)\), assume that the initial data \((\rho _{0},m_{0},u_{0})\) satisfy the following condition:
and the compatibility condition
for some \(g\in L^{2}\). Then there exists a positive constant ε depending only on λ, μ, γ, α, Ω, M, ρ̄ and m̄ such that if
then the slip problem (1.1)–(1.5) has a unique global classical solution \((\rho ,m,u)\) in \(\Omega \times (0,\infty )\) satisfying
In addition, the following large-time behavior
holds for any \(2< q<\infty \).
With (1.14) at hand, we are able to obtain the following large-time behavior of the gradient of the pressure when vacuum states initially appear. It was just a parrel result, which was first established by Li and his collaborators in [6].
Theorem 1.2
Under the conditions of Theorem 1.1, further assume that \(P_{\infty}>0\) and there exists some point \(x_{0}\in \Omega \) such that \(P_{0}(x_{0})=0\). Then the unique global classical solution \((\rho ,m,u)\) to the problem (1.1)–(1.5) obtained in Theorem 1.1has to blow up as \(t\to \infty \) in the sense that for any \(3< r<\infty \),
Remark 1.1
When \(\alpha \le 1\) and \(\gamma >1\), it is easy to show that there exist \(0< C_{i}<1\) (\(i=1,2\)) depending on ρ̄, m̄, \(\rho _{\infty}\) and \(m_{\infty}\), such that the following formula holds
Now, we give some comments on the analysis of this paper. Compared with the bounded domains, because the domain is unbounded, we need to overcome two additional difficulties. First, thanks to [33] (see Lemma 2.6), we can control ∇u by means of divu and curlu, the other one is how to control the boundary integrals, especially (see (3.23)),
In fact, thanks to
and divergence theorem, we can control it.
Next, denote by
and
the material derivative of v and the effective viscous flux, respectively. Then the equation (1.1)3 can be written as
which together with the boundary condition (1.4) implies that one can treat (1.1)3 as a Helmholtz–Wyle decomposition of \((\rho +m)\dot{u,}\) which makes it possible to estimate ∇F and \(\nabla\operatorname{curl}u\). Finally, whereas \(u\cdot n=0\) on ∂Ω, we have
which together with \(\operatorname{curl}u\times n=0\) on ∂Ω is the key to estimating the integrals on the boundary ∂Ω.
2 Preliminaries
In this section, we will recall some known facts and elementary inequalities which will be used frequently later. First, we can get the local existence of strong and classical solutions (see [17]).
Lemma 2.1
Suppose that Ω satisfies the condition of Theorem 1.1, and \((\rho _{0},m_{0},u_{0})\) satisfies (1.7), (1.8) and (1.10). Then there exists a small time \(T_{0}>0\) and a unique strong solution \((\rho ,m,u)\) to the problem (1.1)–(1.5) on \(\Omega \times (0,T_{0}]\) satisfying for any \(\tau \in (0,T_{0})\),
where \(q\in (3,6)\) and \(p_{0}=\frac{9q-6}{10q-12}\in (1,\frac{7}{6})\).
Second, the following Gagliardo–Nirenberg inequality (see [28]) will be used frequently later.
Lemma 2.2
Let Ω be the exterior of a simply connected domain D in \(\mathbb{R}^{3}\). For any \(f\in H^{1}(\Omega )\) and \(g\in L^{q}(\Omega )\cap D^{1,r}(\Omega )\), there exist some generic constants \(C>0\), which may depend on p, q, and r such that
for \(p\in [2,6]\), \(q\in (1,\infty )\), and \(r\in (3,\infty )\).
Then, to get the uniform (in time) upper bound of the density ρ and m, we need the following Zlotnik inequality, which was first used in Huang–Li–Xin [17].
Lemma 2.3
([41])
For \(g\in C(R)\) and \(y,b\in W^{1,1}(0,T)\), assume that the function y satisfies
If \(g(\infty )=-\infty \) and
for all \(0\le t_{1}< t_{2}\le T\) with some \(N_{0}\ge 0\) and \(N_{1}\ge 0\), then
where ζ̂ is a constant such that
Next, thanks to [1, 33], we have the following two lemmas.
Lemma 2.4
Assume that \(D\subset \mathbb{R}^{3}\) is a simply connected bounded domain with \(C^{k+1,1}\) boundary ∂D, \(1< q<+\infty \) and a integer \(k\ge 0\), then for \(v\in W^{k+1,q}(D)\) with \(v\cdot n=0\) on ∂D, there exists a constant \(C=C(q,k,D)\) such that
If \(k=0\), it holds that
Lemma 2.5
Assume that \(D\subset \mathbb{R}^{3}\) is a bounded domain, and its \(C^{k+1,1}\) boundary only has a finite number of two-dimensional connected components. For the integer \(k\ge 0\) and \(1< q<\infty \), and for \(v\in W^{k+1,q}(D)\) with \(v\times n=0\) on ∂D, then exists a positive constant C depending only on q, k, Ω such that
If D has no holes, then
The following conclusion is shown in [1, 33].
Lemma 2.6
Assume that Ω is the exterior of a simply connected domains \(D \subset \mathbb{R}^{3}\) with \(C^{1,1}\) boundary. Then for \(v\in D^{1,q}(\Omega )\) with \(v\cdot n=0\) on ∂Ω, it holds that
and
Due to [24], we obtain the following fact.
Lemma 2.7
Suppose that Ω satisfies the conditions in Lemma 2.6, for any \(v\in W^{1,q}(\Omega )\) (\(1< q<+\infty \)) with \(v\times n=0\) on ∂Ω, it holds that
By Lemmas 2.4–2.7, we can get the following result (see [6]).
Lemma 2.8
Let Ω be the exterior of a simply connected domain \(D\subset \mathbb{R}^{3}\) with smooth boundary. For any \(p\in [2,6]\) and integer \(k\ge 0\), and every \(v\in \{D^{k+1,p(\Omega )}\cap D^{1,2}(\Omega ) \mid v(x,t)\to 0\textit{ as } |x|\to \infty \}\) with \(v\cdot n|_{\partial \Omega}=0\) or \(v\times n|_{\partial \Omega}=0\), then there exists some positive constant C depending only on p, k, and D such that
Then we recall the following Beale–Kato–Majda-type inequality with respect to the slip boundary condition (1.4), which was first proved in [3, 22] when \(\operatorname{div}u\equiv 0\), it can estimate \(\|\nabla u\|_{L^{\infty}}\).
Lemma 2.9
([6])
Assume that \(u\cdot n=0\), \(\operatorname{curl}u\times n=0\), \(\nabla u\in W^{1,q}\), for \(3< q<\infty \), then there exists a constant \(C=C(q)\) such that the following estimate holds
Consider the Neumann boundary value problem
Indeed, the problem is equivalent to
Lemma 2.10
For systems (2.11), we have
-
(1)
For some \(f\in L^{q}\), \(q\in (1,\infty )\), then there exists a unique (modulo constants) solution \(v\in D^{1,q}\) such that
$$ \Vert \nabla v \Vert _{L^{q}(\Omega )}\le C(q,\Omega ) \Vert f \Vert _{L^{q}}. $$ -
(2)
For some \(f\in W^{k,q}\), \(q\in (1,\infty )\), \(k>1\), then \(\nabla F\in W^{k,q}\) and
$$ \Vert \nabla v \Vert _{W^{k,q}}\le C \Vert f \Vert _{W^{k,q}}. $$
Finally, we give the following conclusions for F and curlu, whose proof is in [6]. We sketch it here for completeness.
Lemma 2.11
Let \(\Omega \subset \mathbb{R}^{3}\) be an exterior domain of some simply connected bounded domain with smooth boundary. For any \(2\le p\le 6\) and \(q\in (1,\infty )\), suppose that \((\rho ,m,u)\) is a smooth solution of (1.1) with the boundary condition (1.4), then there exists a positive constant C depending only on p, q, λ, μ, and Ω such that
Moreover,
Proof
First, due to (1.1)3, it is easy to find that F satisfies
It follows from Lemma 2.10 that
and
Due to (1.18) and (1.4), from \(\operatorname{div}\operatorname{curl}u=0\), Lemma 2.7 and (2.18), we get
By virtue of Lemma 2.8, (1.18), (2.19), and (2.20), it indicates that
By (2.1) and (2.20), we can obtain
for any \(2\le p\le 6\).
Employing (1.17), (2.1), (2.18) and (2.22), one has
and
Combining Lemma 2.6 with (2.1), (2.18), and (2.25) gives that
Thus, (2.18), (2.22), (2.23), (2.25) and (2.26) yields the desired result of Lemma 2.11. □
3 A priori estimates (i): lower order estimates
Assume that Ω is the exterior of a simply connected domain \(D \subset \mathbb{R}^{3}\). Choosing a positive real number R such that \(\bar{D}\subset B_{R}\), one can extend the unit outer normal n to Ω as
We will establish some necessary a priori bounds for smooth solutions of the problem (1.1)–(1.5) to extend the local classical solution guaranteed by Lemma 2.1. Thus, let \(T>0\) be a fixed time and \((\rho ,m,u)\) be the smooth solution to (1.1)–(1.5) on \(\Omega \times (0,T]\) with smooth initial data \((\rho _{0},m_{0},u_{0})\) satisfying (1.9) and (1.10). To get the estimates of the obtained solution, set \(\sigma (t)\triangleq \min \{1,t \}\) and define
and
Then, to get the existence of a global classical solution of (1.1)–(1.5), we can get the following proposition.
Proposition 3.1
Under the conditions of Theorem 1.1, there exists a positive constant ε depending only on λ, μ, γ, α, Ω, ρ̄, \(\bar{m,}\) and M such that if \((\rho ,m,u)\) is a smooth solution of (1.1)–(1.5) on \(\Omega \times (0,T]\) satisfying
then
provided \(C_{0}\le \varepsilon \).
Proof
Proposition 3.1 is deduced from Lemmas 3.4–3.7. □
First, we start with the standard energy estimate of \((\rho ,m,u)\).
Lemma 3.2
Suppose that \((\rho ,m,u)\) is a smooth solution of (1.1)–(1.5) on \(\Omega \times (0,T]\). Then there is a positive constant C depending only on λ, μ, and Ω such that
Proof
First, due to \(-\Delta u=-\nabla\operatorname{div}u+\nabla \times\operatorname{curl}u\), we rewrite the third equation of (1.1) as
Multiplying (3.8) by u and integrating the resultant equation over Ω, we obtain that
Multiplying (1.1)1 by \((\int _{{\rho _{\infty}}}^{\rho} \frac{P(s,m)-P(\rho _{\infty},m)}{s^{2}}\,ds + \frac{P(\rho ,m)-P(\rho _{\infty},m)}{\rho} )\) and using (1.4), we have
By the same way, (1.1)2 shows that
Combining (3.9), (3.10), and (3.11), we have
Integrating (3.12) over \((0,T]\) and using (2.7), we find (3.7). This completes the proof of Lemma 3.2. □
Lemma 3.3
Suppose \((\rho ,m,u)\) is a smooth solution of (1.1)–(1.5) satisfying (3.5) on \(\Omega \times (0,T]\). Then there is a positive constant C depending on λ, μ, γ, α, ρ̄, m̄, M, and Ω such that
and
Proof
Motivated by Hoff [16] and Cai–Li–Lü [6], for \(h\ge 0\), multiplying (1.1)3 by \(\sigma ^{h}\dot{u}\) and then integrating it over Ω lead to
Using (1.19) and the fact that \(\operatorname{div}(u\cdot \nabla u)=\nabla u:\nabla u+u\cdot \nabla\operatorname{div}u\), a direct calculation gives
For the boundary term in the first inequality on the right-hand side of (3.16), it follows from (1.17), (2.12), (3.5), and Young’s inequality that
Notice that \(\operatorname{curl}(u\cdot \nabla u)=\nabla u^{i}\times \nabla _{i}u+u\cdot \nabla\operatorname{curl}u\), by (1.4), we have
Finally, a direct calculation leads to
where we have used the fact that
Combining (3.15) and (3.16)–(3.18) gives that for enough small δ.
Integrating (3.19) over \((0,T]\), by Lemma 2.6, (3.5) and (3.7), for \(h\ge 1\), we have
where we have used \(\int _{0}^{T}h\sigma ^{h-1}\sigma '\|P-P_{\infty}\|_{L^{2}}^{2}\,dt \le CC_{0}\). Choosing \(h=1\) and using (3.5) and (3.7), we get (3.13).
Now, we prove (3.14). Applying the operator \(\sigma ^{h}\dot{u}^{j}[\partial /\partial t+\operatorname{div}(u\cdot )]\) to \(\text{(1.18)}^{j}\), summing all the equalities with respect to j and integrating over Ω, we obtain
For the term \(J_{1}\), a direct computation shows that
Setting \(u^{\bot}\triangleq -u\times n\), we have \(u=u^{\bot}\times n\). Applying (2.12), (2.14), we can estimate the three boundary terms as
where we have used
Similarly, we have
It follows from (2.12), (2.14), and (3.21)–(3.23) that
For the term \(J_{2}\), a direct computation yields
Combining \(u=u^{\bot}\times n\) and (1.4) gives
which together with (2.7) and (3.1) implies
Putting (3.24), (3.25), and (3.26) into (3.20), for a enough small δ, we obtain
Integrating (3.27) over \((0,T]\) and using (2.12) and (3.5), when \(h\ge 3\), we have
where in the last inequality, we have used
Then taking \(h=3\) and choosing enough small δ, we obtain (3.14). □
Lemma 3.4
Suppose that \((\rho ,m,u)\) is a smooth solution of (1.1)–(1.5) on \(\Omega \times (0,T]\) satisfying (3.5). Then there exists a positive constant C depending only on λ, μ, ρ̄, m̄, M, and Ω such that
provided \(C_{0}\le \varepsilon _{1}\).
Proof
Taking \(h=0\) in (3.19), integrating over \((0,\sigma (T)]\), and using Lemma 2.6, (2.16), (3.5), and (3.7), we can obtain
Choosing δ small enough, (3.30) gives
provided \(C_{0}\le \varepsilon _{1}\triangleq \{1,\frac{M}{4C}, \frac{1}{4MC} \}\). □
Lemma 3.5
Suppose that \((\rho ,m,u)\) is a smooth solution of (1.1)–(1.5) on \(\Omega \times (0,T]\) satisfying (3.5). Then there exists a positive constant C depending only on λ, μ, ρ̄, m̄, M and Ω such that
Proof
Taking \(h=1\) in (3.27), and integrating over \((0,\sigma (T)]\), by (3.5), (3.29) and (2.16), we have
which gives (3.31) when we choose enough small δ. □
Lemma 3.6
If \((\rho ,m,u)\) is a smooth solution of (1.1)–(1.5) on \(\Omega \times (0, T]\) satisfying the assumption (3.5), then it holds that
Proof
A direct computation shows that
which indicates that
Combining (3.34), (2.14), and (3.5) with (3.7) implies that
which yields (3.32) when we choose enough small δ. □
Lemma 3.7
Assume that \((\rho ,m,u)\) is a smooth solution of (1.1)–(1.5) on \(\Omega \times (0, T]\) satisfying (3.5). Then there exists a positive constant C depending only on λ, μ, γ, α, M, Ω, \(\bar{\rho ,}\) and m̄ such that
provided \(C_{0}\le \varepsilon _{2}\).
Proof
By (2.16), (3.5), (3.7), and (3.32), it holds that
which together with (3.13) and (3.14) gives
It follows from (2.16), (3.5), (3.7), and (3.29) that
On the other hand, using (3.7), (3.36) and Young’s inequality, we can get
By (3.36)–(3.39), we can obtain
which gives (3.35) provided \(C_{0}\le \varepsilon _{2}\triangleq \{\varepsilon _{1}, ( \frac{1}{C (\bar{\rho},\bar{m},M )} )^{6} \}\). □
To get all the higher-order estimates and to extend the classical solution globally, we must derive a uniform (in time) upper bound of the density.
Lemma 3.8
If \((\rho ,m,u)\) is a smooth solution of (1.1)–(1.5) on \(\Omega \times (0, T]\) satisfying (3.5), then there exists a positive constant ε depending only on λ, μ, γ, α, \(\rho _{\infty}\), \(m_{\infty}\), Ω, M, \(\bar{\rho ,}\) and m̄ such that
provided \(C_{0}\le \varepsilon \).
Proof
First, the equations (1.1)1 and (1.1)2 can be rewritten as
where \(D_{t}(\rho +m)\triangleq (\rho +m)_{t}+u\cdot \nabla (\rho +m)\), \(g( \rho +m)\triangleq -\frac{\rho +m}{2\mu +\lambda}(P-P_{\infty})\), and \(b(t)\triangleq -\frac{1}{2\mu +\lambda}\int _{0}^{t}(\rho +m)F\, d\tau \). On the one hand, for all \(0\le t_{1}\le t_{2}\le \sigma (T)\), one deduces from (2.2), (2.12), (2.14), (3.5), (3.29), and (3.31) that
From Lemma 2.3, we choose \(N_{1}=0\), \(N_{0}=C(\bar{\rho}+\bar{m},M)C_{0}^{\frac{1}{16}}\), and \(\hat{\zeta}=\bar{\rho}+\bar{m}\) and then we use (3.42) to get
provided
On the other hand, for \(\sigma (T)\le t_{1}\le t_{2}\le T\), it follow from (2.2), (2.12), (2.14), and (3.5) that
Now, choosing \(N_{0}=CC_{0}\), \(N_{1}=\frac{1}{2\mu +\lambda}\) in (2.3) and setting \(\hat{\zeta}=\bar{\rho}+\bar{m}\) in (2.4), it gives that for all \(\zeta \ge \hat{\zeta}=\bar{\rho}+\bar{m}\),
which together with Lemma 2.3, (3.43), and (3.44) implies
provided
The combination of (3.43) with (3.45) completes the proof of Lemma 3.8. □
4 A priori estimates (ii): higher order estimates
Suppose that \((\rho ,m,u)\) is a smooth solution of (1.1)–(1.5). To extend the classical solution globally in time, assume that (3.46) holds, and the positive constant C may depend on
for besides λ, μ, γ, α, M, Ω, M, \(\bar{\rho ,}\) and m̄, where \(g\in L^{2}(\Omega )\) is gives as in (1.10), we can get some necessary higher-order estimates.
Lemma 4.1
There exists a positive constant C, such that
Proof
By (3.19), (3.38), (3.39) and Lemma 2.6, it gives
which together with Growall’s inequality yields that
Choosing \(h=0\) in (3.27), we deduce from (2.12), (2.16), and (4.3) that
Then choosing δ small enough, it gives (4.1). Observe that for \(2\le p\le 6\), it indicates that
Integrating the above equality over Ω and using (2.12) imply that
Moreover, by Lemma 2.8, (1.17), (2.12), and (2.16), for any \(2\le p\le 6\), we have that
Next, it follows from (2.2), (1.17), (2.12), (2.13), (3.14), and (4.1) that
By Lemma 2.9, (4.5) and (4.6), we get
Combining (4.7) with (4.4) yields
And then by Gronwall’s inequality and (4.1), we obtain
Moreover, (4.7) and (4.8) imply that
Using the above inequality, (4.4) and (4.9), when \(p=2\), yields that
which together with (4.1), (4.5), and (4.8) gives
Hence, we finish the proof of Lemma 4.1. □
Lemma 4.2
There exists a constant C such that
Proof
By Lemma 4.1, a simple computation shows that
and
so we have (4.10). Using (1.1)1, (1.2)2, and (4.2), it shows that
where in the last inequality,we have used the fact that
for any \(p\in [2,6]\) by (2.19)–(2.22) and (1.17).
Employing Gronwall’s inequality, (4.1), (4.2), and (4.12) leads to
Hence,
Therefore, the proof of Lemma 4.2 is completed. □
Lemma 4.3
There exists a constant C such that
Proof
Using (1.1)1, (1.1)2, we have
which together with (4.2) and (4.11) gives
Combining (4.17) with (4.2), (4.11) implies
Due to the fact that \(P_{t}+u\cdot \nabla P+\gamma \rho ^{\gamma}\operatorname{div}u+\alpha m^{ \alpha}\operatorname{div}u=0\), we have
and
By applying (4.18)–(4.21), we get
Differentiating (1.1)1 and (1.1)2 with respect to t implies
Combining (4.23) with (4.2), (4.10), and (4.22) yields
Hence, it gives that
So, we get (4.15).
Next, differentiating (1.1)3 with respect to t and then multiplying by \(u_{tt}\) yield that
It follows from (1.1)1, (1.1)2, (4.2), (4.10), and (4.15) that
Choosing a suitably small positive constant δ and using (4.24)–(4.27), we have
Integrating (4.28) over (0,T], using (1.1)1, (1.1)2, (4.10), (4.15) and Lemma 2.6 gives
Using (4.29), (4.10) and Gronwall’s inequality, we can obtain (4.16). □
Lemma 4.4
For any \(q\in (3,6)\), there exists a positive constant C such that
where \(p_{0}=(1,\frac{9q-6}{10q-12})\in (1,\frac{7}{6})\).
Proof
By (4.13), (4.2), and (4.11), it gives
where we have used the fact that
Then, we deduce from (4.2), (4.10), (4.16), and (4.32) that
Utilizing (4.2) and (4.15) implies that
where in the first inequality, we have used the a priori estimate similar to (4.5) since
Combining (4.34) with (4.16) implies
It follows from (4.13), (4.1), and (4.11) that
which together with (1.1)1 and (1.1)2 gives
and
Hence, integrating inequality (4.38) over [0,T], by (4.1) and (4.35), we obtain
Applying Gronwall’s inequality to (4.37), we deduce from (4.2) and (4.39) that
and then
It follows from (4.36), (4.39), (4.40), and (4.10) that
We finish the proof of Lemma 4.4. □
Lemma 4.5
There exists a positive constant C such that
for any \(q\in (3,6)\).
Proof
Differentiating (1.1)3 with respect to t twice gives
Then, multiplying (4.42) by \(u_{tt}\) and integrating over Ω, we conclude that
Now, we estimate all terms on the right-hand side of (4.43). First, by (4.2), (4.10), and (4.15), it holds
and
Due to the fact that
Using (4.43)–(4.46) and choosing enough small δ, we obtain
which together with (4.10), (4.15), and (4.16) gives that
Furthermore, it follows from (4.34), (4.16), and (4.48) that
Finally, combining (4.36) with (4.38), (4.16), (4.30), and (4.33) that
which together with (4.48) and (4.49) gives (4.41), and this completes the proof of Lemma 4.5. □
5 Proofs of Theorems 1.1 and 1.2
With the a priori proof in Sect. 3 and Sect. 4 at hand, we prove the main results of this paper in this section.
Proof of Theorem 1.1
By Lemma 2.1, the problem (1.1)–(1.5) has a unique local classical solution \((\rho ,m,u)\) on \(\Omega \times (0,T_{\ast}]\) for some \(T_{\ast}>0\). Now, we will extend the classical solution \((\rho ,m,u)\) globally in time.
First, by (3.2) and (3.3), it is easy to check that
Then, there exists a \(T_{1}\in (0,T_{*}]\) such that
Set
Clearly, \(0< T_{1}\le T^{*}\). And for any \(0<\tau <T\le T^{*}\), one deduces from Lemmas 4.3–4.5 that
where one has taken advantage of the standard embedding:
This particularly yields
Next, we claim that
Otherwise, \(T^{*}<\infty \). By Proposition 3.1, it holds that
We deduce from Lemma 4.4, Lemma 4.5 and (5.4) that \((\rho (x,T^{*}),m(x,T^{*}),u(x,T^{*}) )\) satisfy the initial data condition (1.7)–(1.10), where \(g(x)\triangleq (\rho +m)^{\frac{1}{2}}\dot{u}(x,T^{*})\), \(x\in \Omega \). Hence, Lemma 2.1 shows that there is a \(T^{**}>T^{*}\), such that (5.1) holds for \(T=T^{**}\), which contradicts the definition of \(T^{*}\).
Using Lemma 2.1, Lemma 4.4, Lemma 4.5 and (5.3) indicates that \((\rho ,m,u)\) is the unique classical solution defined on \(\Omega \times (0,T]\) for any \(0< T< T^{*}=\infty \).
Finally, to finish the proof of Theorem 1.1, it remains to prove (1.14). It is easy to have
Multiplying (5.7) by \(4(P-{P}_{\infty})^{3}\), one has
which together with (3.7) and (3.32) yields that
Combining (3.32) with (5.8) leads to
For \(2< q<\infty \), by (5.9), we get
Notice that (3.7) imply
Thus, (1.14) follows provided that
Choosing \(h=0\) in (3.19), integrating it over \((1,\infty )\) and using (2.16), (3.5), (3.7), and (3.32), we get
where \(\phi (t)=\frac{\lambda +2\mu}{2}\|\operatorname{div}u\|_{L^{2}}^{2}+ \frac{\mu}{2}\|\operatorname{curl}u\|_{L^{2}}^{2}\). By (3.7), we obtain that
which together with (5.13) yields (5.12). □
Proof of Theorem 1.2
Now, we will prove Theorem 1.2 by contradiction. Suppose that there exists some constant \(C_{1}>0\) and a subsequence \(\{t_{n_{j}} \}_{j=1}^{\infty}\) with \(t_{n_{j}}\to \infty \) as \(j\to \infty \), such that \(\|\nabla P(\cdot ,t_{n_{j}})\|_{L^{r}}\le C_{1}\). Thanks to (2.2), for \(a=3r/ (3r+4(r-3) )\in (0,1)\), it holds that
which together with (1.14) yields that
On the other hand, since \((\rho ,m,u)\) is a classical solution satisfying (1.1), there exists a unique particle path \(x_{0}(t)\) with \(x_{0}(t)=x_{0}\) such that
Hence, we have
which contradicts (5.15). Then, we get the desired result (1.15). Hence, we complete the proof of Theorem 1.2. □
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Funding
Z. Li is supported by the NSFC (No. 12126316, No. 11931013) and Innovative Research Team of Henan Polytechnic University (No. T2022-7). H. Wang is supported by the National Natural Science Foundation of China (No. 11901066), the Natural Science Foundation of Chongqing (No. cstc2019jcyj-msxmX0167), and projects Nos. 2022CDJXY-001, 2020CDJQY-A040 supported by the Fundamental Research Funds for the Central Universities. D. Zhou was partially supported by the National Natural Science Foundation of China under grant No. 12071113.
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Zilai Li, Hao Liu, Huaqiao Wang and Daoguo Zhou wrote the main manuscript text. All authors reviewed the manuscript.
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Li, Z., Liu, H., Wang, H. et al. Global classical solutions to the viscous two-phase flow model with slip boundary conditions in 3D exterior domains. Bound Value Probl 2023, 46 (2023). https://doi.org/10.1186/s13661-023-01733-2
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DOI: https://doi.org/10.1186/s13661-023-01733-2
MSC
- 35Q35
- 35Q30
- 35A09
- 35B40
Keywords
- Two-phase flow model
- Global existence
- Slip boundary condition
- Exterior domains
- Vacuum
- Large-time behavior