Open Access

On global behavior of weak solutions to the Navier-Stokes equations of compressible fluid for \(\gamma=5/3\)

Boundary Value Problems20152015:176

https://doi.org/10.1186/s13661-015-0443-0

Received: 1 August 2015

Accepted: 18 September 2015

Published: 29 September 2015

Abstract

In this article, we consider the global behavior of weak solutions of the Navier-Stokes equations of a compressible fluid in a bounded domain driven by bounded forces for the adiabatic constant \(\gamma=5/3\). Under the condition of a small mass depending on the given forces, we prove the existence of bounded absorbing sets of weak solutions, and thus we further get global bounded trajectories and global attractors to the weak solutions.

Keywords

weak solutionsbounded absorbing setbounded trajectoriesattractors

MSC

35B4035B4176N99

1 Introduction

In this article, we investigate the global behavior of finite energy weak solutions to the Navier-Stokes equations of a viscous compressible isentropic fluid:
$$\begin{aligned} &\partial_{t}\rho+\operatorname{div}(\rho\mathbf{u})=0, \end{aligned}$$
(1)
$$\begin{aligned} &\partial_{t} (\rho\mathbf{u})+\operatorname{div}(\rho \mathbf{u}\otimes\mathbf{u})+ \nabla P=\mu\Delta\mathbf{u}+(\mu+\lambda)\nabla \operatorname{div}\mathbf{u} +\rho{\mathbf{f}}, \end{aligned}$$
(2)
in \(\Omega\times I\), and with a non-slip boundary condition:
$$ \mathbf{u}(t,x)|_{\partial\Omega}=\mathbf{0}, \quad t\in I\subset \mathbb{R}. $$
(3)
In this article, we always assume that \(\Omega\subset\mathbb{R}^{3}\) is a bounded domain with Lipschitz boundary, and I an open time interval. The unknown functions \(\varrho=\rho(t,x)\) and \(\mathbf{u}= \mathbf{u}(t,x)=(u^{1}(t,x),u^{2}(t,x),u^{3}(t,x))\) represent the density and velocity of fluid, respectively. The external force \({\mathbf{f}}=(f^{1}(t,x),f^{2}(t,x), f^{3}(t,x))\) is given. The pressure takes the form \(P=a\rho^{\gamma}\), where a is a positive constant, and γ the adiabatic constant. \(\mu>0\) and λ are the viscosity constants, satisfying \(3\lambda +2\mu\geq0\).

Next we give the standard definition of finite energy weak solutions to the problem (1)-(3) as in [1, 2].

Definition 1.1

Let \(\gamma>3/2\). we call the couple \((\rho, \mathbf{u})\) a finite energy weak solution to the problem (1)-(3), if it satisfies the following properties:
  • ρ, u enjoy the regularity
    $$ \rho\in L_{\mathrm{loc}}^{\infty}\bigl(I;L^{\gamma}( \Omega)\bigr)\cap L_{ \mathrm{loc}}^{s(\gamma)}\bigl(I;L^{s(\gamma)}(\Omega) \bigr),\qquad u^{i}\in L^{2}_{\mathrm{loc}} \bigl(I;W^{1,2}_{0}(\Omega)\bigr) $$
    (4)
    for \(i=1,2,3\) and \(s(\gamma)=({5\gamma-3})/{3}\).
  • Let the energy E be defined as follows:
    $$ E[\rho,{\mathbf{u}} ](t) =\int_{\Omega}\biggl[ \frac{1}{2}\rho(t,x)\bigl|{\mathbf{u}}(t,x)\bigr|^{2} +\frac{a}{{\gamma-1}} \rho^{\gamma}(t,x) \biggr] \,\mathrm{d}x, $$
    (5)
    then \(E\in L^{1}_{\mathrm{loc}}(I)\) satisfies the following energy inequality in \(\mathcal{D}'(I)\):
    $$ \frac{\mathrm{d}}{\mathrm{d}t}E[\rho,{\mathbf{u}} ](t)+\int_{\Omega}\bigl[\mu\bigl|\nabla\mathbf{u}(t)\bigr|^{2}+(\lambda+\mu) \bigl|\operatorname{div} { \mathbf{u}}(t)\bigr|^{2}\bigr]\,\mathrm{d}x \leq \int_{\Omega}\rho(t){\mathbf{f}}(t)\cdot{{\mathbf{u}}}(t)\,\mathrm{d}x. $$
    (6)
  • Equations (1) and (2) hold in \(D'(I\times \Omega )\); moreover, (1) is satisfied in \(D'(I\times\mathbb{R}^{3})\) provided we prolong \(\rho, \mathbf{u}\) to be zero on \(\mathbb {R}^{3}/\Omega\).

  • Equation (1) is satisfied in the sense of renormalized solutions, i.e.,
    $$ b(\rho)_{t}+\operatorname{div} \bigl(b(\rho)\mathbf{u} \bigr)+\bigl(b'(\rho)\rho-b(\rho)\bigr)\operatorname{div}\mathbf{u}=0 $$
    (7)
    holds in \(D'(I\times\Omega)\) for any b satisfying
    $$ b\in C^{0}\bigl([0,\infty]\bigr)\cap C^{1} \bigl((0,\infty )\bigr),\qquad \bigl|b'(t)\bigr|\leq Ct^{-\lambda_{0}}, \quad t \in(0,1), \lambda_{0}< 1, $$
    (8)
    and
    $$ \bigl|b'(t)\bigr|\leq C t^{\lambda_{1}},\quad t\geq1,\textit{ where }C>0, -1< \lambda_{1}\leq\frac{s(\gamma)}{2}-1. $$
    (9)
The existence of globally defined weak solutions for \(\Omega\subset \mathbb{R}^{3}\) was proved by Lions [3] under the hypothesis that \(\gamma>9/5\). Then, by using the curl-div lemma to subtly derive a certain compactness, and applying Lions’ idea and a technique from [4], Feireisl et al. [1] extended Lions’ existence result to the case \(\gamma> 3/2\). For any \(1\leq\gamma\leq3/2\), a global weak solution still exists when the initial data have a certain symmetry (e.g., spherical, or axisymmetric symmetry); see [4, 5]. The theory of weak solutions is also applied to other models of fluid mechanics; see [610] for examples. In [2, 1113] Feireisl and Petzeltová investigated the global behavior of weak solutions of the problem (1)-(3), and showed the existence of bounded absorbing sets, global bounded trajectories and global attractors to weak solutions of compressible flows for \(\gamma> 5/3\). Jiang et al. [1416] and Wang [17] further generalized their results to the Navier-Stokes-Poisson equations and nematic liquid crystals, respectively. However, it is still an open problem for the case \(\gamma>3/2\). In this article, under the proof-frame of [2, 11], we investigate the global behavior of weak solutions of the problem (1)-(3) for \(\gamma= 5/3\) under the assumption of small mass depending on the given forces. Finally, we mention that, from the definition of renormalized solutions, the total mass m is conserved, i.e.
$$ m=\int_{\Omega}\rho(x,t)\,\mathrm{d}x \mbox{ is independent of }t\in I. $$
(10)

Next we start to state our main results. The first result concerns the existence of bounded absorbing sets of weak solutions to the problem (1)-(3).

Theorem 1.1

Let \(\gamma=5/3\), \(a_{0}>-\infty\), \(I=(a_{0}, \infty)\subset\mathbb{R}\) be an open interval, and the bounded measurable function \({\mathbf{f}}=(f^{1}(t,x),f^{2}(t,x),f^{3}(t,x))\) satisfy
$$ \max_{i=1,2,3} \Bigl\{ \operatorname{ess}\sup _{t\in I,x\in\Omega} \bigl|f^{i}(t,x) \bigr| \Bigr\} \leq K. $$
(11)
Then there exist constants \(m_{0}:=m_{0}(K )\in(0,1)\) and \(E_{\infty}:=E( K)\) satisfying the following property:
For any positive constant \(E_{0}\) and any finite energy weak solution \((\rho,{\mathbf{u}} )\) of the problem (1)-(3), if
$$ \operatorname{ess}\limsup_{t\rightarrow a_{0}}E(t)\leq E_{0}\quad\textit{and}\quad m\leq m_{0}, $$
(12)
then there exists a time point \(T=T(E_{0}, a_{0})\) such that
$$ E(t):=E[\rho,{\mathbf{u}}](t)\leq E_{\infty}\quad\textit{for a.e. }t>T. $$
(13)
Here we explain why our arguments work only for \(\gamma=5/3\). In Feireisl and Petzeltová’s article [2], they deduced the following key estimate:
$$\begin{aligned} &\sup_{t\in[T,T+1]}E(t+) \\ &\quad\leq c(K,m) \Bigl(1+\sup_{t\in[T,T+1]}\sqrt{E(t+)}+\tilde {c}(m) \sup_{t\in[T,T+1]} \bigl\| \varrho(t)\bigr\| _{L^{\gamma}(\Omega)}^{(4\gamma-3)(3(\gamma+\theta -1))} \Bigr), \end{aligned}$$
(14)
where \(c(K,m)\) and \(\tilde{c}(m)\) are two positive constants. Under the condition \(\gamma>5/3\), \((4\gamma-3)/(3(\gamma+\theta -1))<\gamma\), and thus one can apply the Young inequality to the estimate above to deduce
$$ \sup_{t\in[T,T+1]}E(t+)\leq L $$
(15)
for some constant \(L>0\). The local-time boundedness (15) is very important to further deduce the existence of a bounded absorbing set. However, if \(\gamma\leq5/3\), then \((4\gamma-3)/(3(\gamma+\theta -1))\geq\gamma\), and thus the above idea to deduce (15) obviously fails. However, when \(\gamma=5/3\), (14) implies
$$ \sup_{t\in[T,T+1]}E(t+) \leq c(K,m) \Bigl(1+\sup _{t\in[T,T+1]}\sqrt{E(t+)}+\tilde{c}(m) \sup_{t\in[T,T+1]}E(t+) \Bigr). $$
(16)
By careful analyzing the derivation of (15), we observe that \(c(K,m)\) and m converge to zero as \(m\to0\), and thus (15) can be still deduced from (16) provided that the mass is sufficiently small.
Based on Theorem 1.1, we can further get global bounded trajectories of weak solutions to the problem (1)-(3) as in [12], since the family of trajectories generated by the finite energy weak solutions of (1)-(3) defined on I possesses a bounded absorbing set in the energy ‘norm’. To this purpose, we define
$$\begin{aligned} U^{s}[E_{0},\mathcal{F} ](t_{0}, t)={}& \Bigl\{ \bigl(\rho(\tau),\mathbf{q}(\tau) \bigr), \tau\in [0,1] |\rho( \tau)=\rho(t+\tau),\ \mathbf{q}(\tau)=(\rho\mathbf{u}) (t+\tau), \\ &{}\mbox{where }(\rho, \mathbf{u}) \mbox{ is a finite energy weak solution to the} \\ &{}\mbox{problem (1)-(3) on an open interval }I, \mbox{ such that }(t_{0}, t_{0}+1]\subset I, \\ &{}\mathbf{f}\in\mathcal{F}, \operatorname{ess}\limsup_{t\rightarrow t_{0}} E(t)\leq E_{0} \mbox{ and } m \mbox{ satisfy }(12) \Bigr\} . \end{aligned}$$
(17)
Then we have the second result concerning the large-time behavior of the short trajectories defined in (17).

Theorem 1.2

Let \(\gamma=5/3\), \(J_{1}=(0,1)\),
$$ \mathcal{F} \textit{ be bounded subset of the }\bigl(L^{\infty}( \mathbb {R}\times \Omega)\bigr)^{3} $$
(18)
and
$$\begin{aligned} \mathcal{F}^{+}={}& \Bigl\{ \mathbf{f}\big\vert \mathbf{f}=\lim _{\tau _{n}\rightarrow\infty}\mathbf{h}_{n}(t+\tau_{n}, x)\textit{ weak star in }L^{\infty}(\mathbb{R}\times\Omega) \\ &{}\textit{for a certain }\mathbf{h}_{n}\in\mathcal{F} \textit{ and } \tau_{n}\rightarrow\infty \Bigr\} . \end{aligned}$$
(19)
Assume that there exists a certain sequence \(t_{n}\rightarrow\infty\) satisfying
$$\bigl(\rho_{n}(t_{n}+t,x), \mathbf{q}_{n}(t_{n}+t,x) \bigr)\in U^{s}[E_{0}, \mathcal{F} ](a_{0}, t_{n})\quad (a_{0}\in\mathbb{R}), $$
then we can extract a subsequence (not relabeled) such that
$$\begin{aligned}& \rho_{n}(t_{n}+t, x)\rightarrow\bar{\rho}(t, x)\quad \textit{in }L^{5/3}(J_{1}\times \Omega) \textit{ and in }C \bigl(\bar{J}_{1}; L^{\alpha}(\Omega)\bigr)\textit{ for }1\leq \alpha< 5/3, \end{aligned}$$
(20)
$$\begin{aligned}& \mathbf{q}_{n}(t_{n}+t, x)\rightarrow(\bar{\rho}\bar{ \mathbf{u}}) (t, x)\quad\textit{in } L^{p}(J_{1}\times\Omega) \cap C\bigl(\bar{J}_{1}; \bigl(L^{\frac {5}{4}}_{\mathrm{weak} }(\Omega) \bigr)^{3} \bigr), \end{aligned}$$
(21)
and
$$ E\bigl[\rho_{n}(t_{n}+t, x), \mathbf{u}_{n}(t_{n}+t, x)\bigr]\rightarrow E\bigl[\bar{ \rho}(t, x),\bar{\mathbf{u}}(t, x) \bigr]\quad \textit{in }L^{1}(J_{1}) $$
(22)
for any \(p \in [1,\frac{5}{4} )\), where (ρ̄, ) is a finite energy weak solution of the problem (1)-(3) defined on the whole real line \(I=\mathbb{R}\) such that \(E\in L^{\infty}(\mathbb{R})\), \(\int_{\Omega}\bar {\rho}\,\mathrm{d}x= m\), and \(\mathbf{f}\in\mathcal{F}^{+}\).
The theorem above presents that the energy E of finite energy weak solutions defined on \(I=\mathbb{R}\) is uniformly bounded on \(\mathbb{R}\), and thus we can further construct a set of short trajectories to which any finite energy weak solution is asymptotically attracted by Theorem 1.2. To this end, we define
$$ \begin{aligned}[b] \mathcal{A}^{s}[\mathcal{F}]={}& \bigl\{ \bigl(\rho(\tau ),\mathbf {q}(\tau) \bigr)_{\tau\in[0,1]} | \bigl(\rho, \mathbf{q}=(\rho \mathbf{u}) \bigr)\mbox{ is a finite energy weak solution}\\ &{}\mbox{of the problem (1)-(3) on } I=\mathbb {R}, \mbox{with }\mathbf{f}\in\mathcal{F}^{+}, E[\rho,\mathbf{u} ]\in L^{\infty}(\mathbb{R})\\ &{}\mbox{and } m \mbox{ satisfy }(12) \bigr\} . \end{aligned} $$
(23)
Thus, we have the third conclusion as regards a global attractor to the short trajectories of the set \(\mathcal{A}^{s}(\mathcal{F})\) as in [12].

Theorem 1.3

Assume \(\gamma=5/3\) and \(\mathcal{F}\) satisfies (18). Then the set \(\mathcal{A}^{s}[\mathcal{F}]\) is compact in \(L^{5/3}(J_{1}\times \Omega)\times(L^{p}(J_{1}\times\Omega))^{3} \). Moreover, for any \(p\in [1, 5 )\),
$$\begin{aligned} \sup_{(\rho,\mathbf{q} )\in U^{s}[E_{0},\mathcal{F} ](t_{0}, t)} \Bigl[\inf_{(\bar{\rho}, \bar{\mathbf{q}} )\in\mathcal {A}^{s}[\mathcal{F}]}\bigl(\| \rho-\bar{\rho} \|_{L^{5/3}(J_{1}\times \Omega)}\bigr)+\|\mathbf{q}-\bar{\mathbf{q}}\|_{L^{p}(J_{1}\times \Omega)} \Bigr] \rightarrow0, \end{aligned}$$
(24)
as \(t\rightarrow\infty\).
The theorem above shows that the set \(\mathcal{A}^{s}(\mathcal{F})\) is a global attractor to the space of short trajectories; moreover, the set \(\mathcal{A}^{s}(\mathcal{F})\) is nonempty and compact, if \(\mathcal{F}\) is nonempty. Similar to [18], we can further build a set of global trajectories. To this end, we define
$$\begin{aligned} \mathcal{A}[\mathcal{F}]={}& \bigl\{ (\rho,\mathbf{q} )\vert \rho=\rho(0), \mathbf{q}=(\rho\mathbf{u}) (0), \mbox{ where }\rho, \mathbf{u} \mbox{ is a finite energy} \\ &{}\mbox{weak solution of the problem (1)-(3) on } I= \mathbb{R} \\ &{}\mbox{with }\mathbf{f}\in\mathcal {F}^{+}\mbox{ and } E\in L^{\infty}( \mathbb{R}), \mbox{ and } m \mbox{ satisfy }(12)\bigr\} , \end{aligned}$$
(25)
and
$$\begin{aligned} &U[E_{0},\mathcal{F} ](t_{0},t) \\ &\quad= \Bigl\{ (\rho,\mathbf{q} ) (t) \big| (\rho, \mathbf{u} ) \mbox{ is a finite energy weak solution of the problem} \\ &\qquad{}\mbox{(1)-(3) on }I \mbox{ such that }(t_{0}, t]\subset I, \mathbf{f}\in\mathcal{F}\mbox{ and } \operatorname{ess}\limsup_{t\rightarrow t_{0}} E(t)\leq E_{0}, \\ &\qquad{} \mbox{and } m \mbox{ satisfy }(12) \Bigr\} , \end{aligned}$$
(26)
thus we get the fourth result on attractors as in [12].

Theorem 1.4

We redefine the energy E by
$$ E[\rho,{\mathbf{u}}](t)=\int_{\rho(x, t)>0} \biggl[ \frac{1}{2}\frac{| \rho \mathbf{u}|^{2}}{\mathbf{\rho}}(t, x) +\frac{3a}{2}\rho^{5/3}(t, x) \biggr] \,\mathrm{d}x. $$
(27)
Assume that \(\gamma=5/3\) and \(\mathcal{F}\) satisfies (18), then \(\mathcal{A}[\mathcal{F}]\) is compact in \(L^{\alpha}(\Omega) \times( L^{\frac{5}{4}}_{\mathrm{weak}}(\Omega))^{3}\), i.e., for any \(1\leq \alpha < 5/3\) and any \(\phi\in(L^{5}(\Omega))^{3}\),
$$ \sup_{(\rho,\mathbf{q} )\in U[E_{0},\mathcal{F} ](t_{0},t)}\biggl[\inf_{(\bar{\rho},\bar{\mathbf{q}} )\in\mathcal {A}[\mathcal{F}]} \biggl(\|\rho-\bar{\rho}\|_{L^{\alpha}(\Omega)} +\biggl|\int_{\Omega}( \mathbf{q}-\bar{\mathbf{q}} )\cdot\phi\,\mathrm{d}x\biggr| \biggr) \biggr]\rightarrow0 \quad \textit{as } t\rightarrow\infty. $$
(28)

Remark 1.1

It should be noted that the energy \(E(t)\) defined by (27) is equal to (5) a.e. in I (see [18], Lemma 7.18) and (27) is lower semicontinuous (see [18], Proposition 7.21). Then the two conditions ‘\(\operatorname{ess}\limsup_{t\rightarrow a} E(t)\leq E_{0}\)’ and ‘\(\limsup_{t\rightarrow a} E(t)\leq E_{0}\)’ are equivalent, and, thus, the conclusions in Theorems 1.1-1.2 with \(E(t)\) defined by (27) still hold, in particular, we have \(E(t):=E[\rho,\mathbf{u} ](t)\leq E_{\infty}\) for \(t>T\) in Theorem 1.1.

In next section, we use the proof-frame of [2] to prove Theorem 1.1 under the condition of small mass. Once we establish Theorem 1.1, the conclusions in Theorems 1.2-1.4 obviously hold by the standard compactness method as in [1, 12]; hence we omit the proof.

2 Proof of Theorem 1.1

Similar to [2], to get Theorem 1.1, it suffices to obtain the following two results.

Proposition 2.1

Under the hypotheses of Theorem  1.1, let \(m\in(0,1)\) and \((\rho, \mathbf{u} )\) be a renormalized solution of (1)-(3), then the energy E is locally bounded variation on I (being redefined on a set of measure zero if necessary), and
$$ E(t+)=\lim_{s\rightarrow t+}E(s)\leq \lim _{s\rightarrow t-}E(s)=E(t-) \quad\textit{for any } t\in I. $$
(29)
Moreover, there exists a constant \(c(K)\), only depending on K and independent of m, such that
$$ E(t_{2}-)\leq \bigl(1+E(t_{1}+) \bigr)e^{c(K)(t_{2}-t_{1})}-1\quad \textit{for all } 0< t_{1}< t_{2}. $$
(30)

Proposition 2.2

Under the assumptions of Theorem  1.1, there exists a constant \(m_{0}\in(0,1)\) such that for any \(m\in(0,m_{0})\) there exists a constant \(L:=L( K )\) enjoying the following property:

If
$$ E\bigl((T+1)-\bigr)>E(T+)-1 \quad\textit{for some } T\in I, $$
(31)
then
$$ \sup_{t\in(T,T+1)}E(t+)\leq L. $$
(32)

For completeness of this article, we provide the proof of Theorem 1.1 in detail, based on Propositions 2.1-2.2. It is easy to see that there exists \(T=T(E_{0}, a_{0})>a_{0}\) satisfying \(E(T-)>E((T-1)+)-1\). Indeed if it fails, then, when the t is sufficiently large, the energy would be negative. This contradicts the fact that the energy is non-negative. Therefore \(E(t_{0})\leq L\) for some \(t_{0}< T\), where L is defined as in Proposition 2.2.

Next we claim that
$$ E\bigl((t_{0}+n)+\bigr)\leq L \quad\mbox{for any } n \geq0, $$
(33)
By induction, we assume \(E((t_{0}+n)+)\leq L\). Making use of (29) and Proposition 2.2, either
$$ \sup_{t\in(t_{0}+n,t_{0}+n+1)}E(t+)\leq L, $$
which implies \(E((t_{0}+n+1)-)\leq L\), or
$$E\bigl((t_{0}+n+1)+\bigr)\leq E\bigl((t_{0}+n+1)-\bigr)\leq E\bigl((t_{0}+n)+\bigr)-1\leq L-1. $$
Consequently, in view of (33) and Lemma 2.1, we take the value
$$E_{\infty}=(1+L)e^{c(K)}-1, $$
to obtain Theorem 1.1. This completes the proof of Theorem 1.1.

Next we turn to strictly show the two propositions above. We mention that all the estimate constants appearing in this section is independent of m.

2.1 Proof of Proposition 2.1

Let \(E_{1}(t)\) satisfy
$$ \frac{\mathrm{d}}{\mathrm{d}t}E_{1}(t)+\int_{\Omega}\mu |\nabla {\mathbf{u}}|^{2}+(\lambda+\mu)|\operatorname{div} {\mathbf{u}}|^{2} \,\mathrm{d}x= \int_{\Omega}\rho{\mathbf{f} \cdot{{\mathbf{u}}}}\,\mathrm{d}x\quad\mbox{a.e. for } t\in I, $$
(34)
then \(E_{2}:=(E-E_{1})\in L^{1}_{\mathrm{loc}}(I)\). In view of (6), we get
$$ \frac{\mathrm{d}}{\mathrm{d}t}E_{2}(t)\leq 0\quad\mbox{in } \mathcal{D}'(I). $$
(35)
Hence E is the sum of ‘an absolutely function’ and ‘a nonincreasing function’, and thus, E is a continuous function except a countable set of points in which (29) holds. In addition, using the condition (11), we can control the right-hand side of (6) as follows:
$$\begin{aligned} \int_{\Omega}\rho{\mathbf{f}\cdot{{\mathbf{u}}}} \,\mathrm{d}x&\leq K \biggl(\int_{\Omega}\rho\,\mathrm{d}x \biggr)^{\frac{1}{2}} \biggl(\int_{\Omega}\rho|{\mathbf{u}}|^{2} \,\mathrm{d}x \biggr)^{\frac{1}{2}} \leq\sqrt{2m}K \biggl(1+\int _{\Omega}\rho|{\mathbf{u}}|^{2} \,\mathrm{d}x \biggr) \\ &\leq\sqrt{2m}K\bigl(1+2E(t)\bigr)\leq2\sqrt{2}K \bigl(1+E(t) \bigr):=c( K) \bigl(1+E(t) \bigr), \end{aligned}$$
(36)
where we have used the condition \(m\in(0,1)\). Thus, using the Gronwall lemma, we immediately get (30), and we complete the proof of Proposition 2.1.

2.2 Proof of Proposition 2.2

Before further providing the proof of Proposition 2.2, we shall establish the following four auxiliary lemmas.

Lemma 2.1

Under the hypotheses of Theorem  1.1 and (31), let \(m\in(0,1)\), then
$$ \int_{T}^{T+1}\bigl\| {\mathbf{u}}(t) \bigr\| _{W_{0}^{1,2}(\Omega)}^{2} \,\mathrm{d}t\leq c_{1} \biggl(1+\int _{T}^{T+1}\bigl\| \rho(t)\bigr\| _{L^{\frac{3}{2}}(\Omega)}\,\mathrm{d}t \biggr) $$
(37)
holds for a constant \(c_{1}=c_{1}(K)\).

Proof

Exploiting (31), the energy inequality (6), the embedding theorem \(W^{1,2}(\Omega)\subset L^{6}(\Omega)\), and the Poincaré inequality, we can estimate
$$\int_{\Omega}\mu\bigl|\nabla{\mathbf{u}}(t)\bigr|^{2} \,\mathrm{d}x \leq c_{1,1} \biggl(1+\int_{T}^{T+1} \int_{\Omega}\rho|\mathbf {u}|\,\mathrm{d}x\,\mathrm {d}t \biggr). $$
On the other hand, we can use the Hölder inequality and the condition \(m\in(0,1)\) to estimate
$$ \int_{\Omega}\rho|{\mathbf{u}}|\,\mathrm{d}x\leq\sqrt{m} \biggl( \int_{\Omega}\rho|{\mathbf{u}}|^{2} \,\mathrm{d}x \biggr)^{\frac{1}{2}}\leq\|\rho\|_{L^{3/2}(\Omega)}^{1/2}\|{\mathbf{u}} \|_{L^{6}(\Omega)}. $$
Consequently, we immediately get the desired result by using the embedding theorem again. □

Lemma 2.2

Under the assumptions of Theorem  1.1 and (31), there exists a constant \(m_{0}\in(0,1)\) depending on K such that, for any
$$ m\in(0,m_{0}], $$
(38)
we have
$$ E(t+)\leq c_{2} \biggl(1+\int_{T}^{T+1} \bigl\| \rho(s)\bigr\| _{L^{5/3}(\Omega)}^{5/3} \,\mathrm{d}s \biggr) \quad\textit{for any } t\in[T, T+1] $$
(39)
for some constant \(c_{2}=c_{2}(K )\).

Proof

We integrate (30) for the choice \(t_{2}=T+1\) with respect to \(t_{1}\) to obtain
$$E\bigl((T+1)-\bigr)\leq c_{2,1} \biggl(1+\int_{T}^{T+1}E(s) \,\mathrm{d}s \biggr). $$
In addition,
$$ E(T+)< E\bigl((T+1)-\bigr)+1\leq c_{2,2} \biggl(1+\int _{T}^{T+1}E(s)\,\mathrm {d}s \biggr). $$
(40)
Thus, we can take \(t_{1}=T\) in (30) and use (40) to obtain
$$E(T+) \leq c_{2,3} \biggl(1+\int_{T}^{T+1}E(s) \,\mathrm{d}s \biggr) \quad\mbox{for any }t\in[T,T+1). $$
Now, exploiting the Hölder inequality and Lemma 2.1, we can infer that
$$\begin{aligned} \int_{T}^{T+1}\int_{\Omega}\rho| \mathbf{u}|^{2}\,\mathrm{d}x\,\mathrm{d}t &\leq\sup_{t\in[T,T+1)} \bigl\| \rho(t)\bigr\| _{L^{3/2}(\Omega)}\int_{T}^{T+1}\| \mathbf {u}\|_{W^{1,2}_{0}(\Omega)}^{2}\,\mathrm{d}s \\ &\leq c_{2,4}\sup_{t\in[T,T+1]}\bigl\| \rho(t)\bigr\| _{L^{3/2}(\Omega)} \biggl(1+ \int_{T}^{T+1} \|\rho\|_{L^{3/2}(\Omega)} \,\mathrm{d}t \biggr). \end{aligned}$$
We can use the interpolation inequality to get
$$\|\rho\|_{L^{3/2}(\Omega)}\leq\|\rho\|_{L^{1}(\Omega)}^{1/6}\|\rho\| ^{5/6}_{L^{5}/3(\Omega)}, $$
and thus
$$\int_{T}^{T+1}\int_{\Omega}\rho| \mathbf{u}|^{2}\,\mathrm{d}x\,\mathrm{d}t \leq c_{2,5}\sup _{t\in[T,T+1]}E(t+)^{1/2} \biggl(1+ m^{1/6}\int _{T}^{T+1} \bigl\| \rho(s)\bigr\| _{L^{5/3}(\Omega)}^{5/6} \,\mathrm{d}s \biggr). $$
Hence we further have
$$\begin{aligned} \sup_{t\in[T,T+1]}E(t+) \leq{}&c_{2,6} \biggl[1+ \int _{T}^{T+1}\bigl\| \rho(t)\bigr\| _{L^{{5/3}}(\Omega )}^{5/3}\,\mathrm{d}s \\ &{} +\sup_{t\in[T,T+1]}E(t+)^{1/2} \biggl(1+ m^{1/6}\int_{T}^{T+1} \|\rho \|_{L^{5/3}(\Omega)}^{5/6}\,\mathrm{d}t \biggr) \biggr]. \end{aligned}$$
Consequently, there exists a sufficiently small constant \(m_{0}\in(0,1)\) dependent on K such that, for any \(m\in(0,m_{0}]\), (39) holds. □

Lemma 2.3

Let \((\rho, \mathbf{u})\) be a finite energy weak solutions to the problem (1)-(3) and
$$S_{\varepsilon}[v]=\vartheta_{\varepsilon}\ast v, \quad\textit{where } \vartheta _{\varepsilon}=\vartheta_{\varepsilon}(x)\textit{ is a regularizing sequence}. $$
Then
$$ \partial_{t}S_{\varepsilon}\bigl[b(\rho )\bigr]+ \operatorname{div}\bigl(S_{\varepsilon}\bigl[b(\rho)\bigr]{\mathbf{u}}\bigr) +S_{\varepsilon}\bigl[\bigl(b'(\rho)\rho-b(\rho)\bigr) \operatorname{div} {\mathbf{u}} \bigr]=r_{\varepsilon}$$
(41)
a.e. in \(I\times\mathbb{R}^{3}\). Moreover, if
$$b(\rho)\textit{ is in }L^{\infty}_{\mathrm{loc}}\bigl( \mathbb{R}^{+},L^{\beta}(\Omega)\bigr),\quad \beta\geq2, $$
then
$$ r_{\varepsilon}\rightarrow0 \textit{ in }L^{2}_{\mathrm {loc}} \bigl(\mathbb{R}^{+}; L^{\alpha}(\Omega)\bigr)\textit{ for }\varepsilon \rightarrow0 \textit{ with }\alpha=\frac{2\beta}{\beta+2}. $$
(42)

Proof

Please, refer to [2], Lemma 2.1 or [18], Lemmas 6.7-6.9. □

Lemma 2.4

Let \(p,r\in(1,\infty)\) be given numbers, then there exists a bounded linear operator  \(\mathcal{B}\),
$$\begin{aligned} &{\mathcal{B}}=[{\mathcal{B}}_{1},{\mathcal{B}}_{2},{ \mathcal{B}}_{3}]: \biggl\{ f\in L^{p}(\Omega) \Big|\int _{\Omega}f\,\mathrm{d}x=0 \biggr\} \mapsto \bigl[W_{0}^{1,p}( \Omega)\bigr]^{3}, \\ &\bigl\| {\mathcal{B}}\{f\}\bigr\| _{W_{0}^{1,p}(\Omega )}\leq c_{3}(p,\Omega)\|f \|_{L^{p}(\Omega)} \end{aligned}$$
(43)
such that \({\mathbf{v}}:={\mathcal{B}}\{f\}\) satisfies
$$ \operatorname{div} {\mathbf{v}}=f\quad\textit{a.e. in }\Omega, { \mathbf{v}}|_{\partial\Omega}=0. $$
(44)
In addition, if \(f\in L^{r}(\Omega)\) can be written by
$$f=\operatorname{div} \mathbf{h}\quad \textit{for a certain } \mathbf{h}\in \bigl[L^{r}(\Omega)\bigr]^{3}, \mathbf{h} \cdot{\mathbf{n}}|_{\partial\Omega}=0, $$
then
$$ \bigl\| {\mathcal{B}}\{f\}\bigr\| _{L^{r}(\Omega)}\leq c_{4}(p, \gamma,\Omega)\|{\mathbf{h}}\|_{L^{r}(\Omega)}. $$
(45)

Proof

The bounded linear operator \({\mathcal{B}} \) was first considered by Bogovskii [19], please refer to [20], Proposition 2.1, for a detailed proof. □

We are now in the position to prove Proposition 2.2. Let \(0\leq\psi\leq1\), \(\psi\in{\mathcal{D}}(T,T+1)\), and \(S_{\varepsilon}\) are the smoothing operators given by Lemma 2.3. We consider test functions
$$\varphi_{i}(t,x)=\psi(t){\mathcal{B}}_{i} \biggl\{ S_{\epsilon}\bigl[b(\rho)\bigr]-\frac{1}{|\Omega|}\int_{\Omega}S_{\epsilon}\bigl[b(\rho)\bigr]\,dx \biggr\} , \quad i=1,2,3, $$
where
$$ b\in C^{1}(R), \qquad b(z)=z^{1/15}\quad\mbox{for }z\geq1 . $$
(46)
Taking the \(\varphi_{i}\) as test functions for (2) and exploiting Lemmas 2.3 and 2.4, we can obtain the following identity:
$$\begin{aligned} &a\int_{T}^{T+1}\int _{\Omega}\psi\rho^{5}/3 S_{\epsilon}\bigl[b(\rho) \bigr]\,\mathrm{d}x\,\mathrm{d}t \\ &\quad=\int_{T}^{T+1}\psi \biggl(\int _{\Omega}a\rho^{5}/3\,\mathrm{d}x \biggr) \frac {1}{|\Omega|}\int_{\Omega}S_{\epsilon}\bigl[b(\rho) \bigr] \,\mathrm{d}x )\,\mathrm{d}t \\ &\qquad{}+(\lambda+\mu) \int_{T}^{T+1}\int _{\Omega}\psi S_{\epsilon}\bigl[b(\rho)\bigr] \operatorname{div} {\mathbf{u}}\,\mathrm{d}x\,\mathrm{d}t \\ &\qquad{}- \int_{T}^{T+1}\int_{\Omega}\psi_{t}\rho u^{i}{\mathcal {B}}_{i} \biggl\{ S_{\epsilon}\bigl[b(\rho)\bigr]-\frac{1}{|\Omega|}\int_{\Omega}S_{\epsilon}\bigl[b(\rho)\bigr]\,\mathrm{d}x \biggr\} \,\mathrm{d}x\,\mathrm{d}t \\ &\qquad{}+\mu \int_{T}^{T+1}\int _{\Omega}\psi\partial_{x_{j}} u^{i} \partial_{x_{j}}{\mathcal{B}}_{i} \biggl\{ S_{\epsilon}\bigl[b(\rho)\bigr]-\frac {1}{|\Omega|}\int_{\Omega}S_{\epsilon}\bigl[b(\rho)\bigr]\,\mathrm{d}x \biggr\} \,\mathrm{d}x\,\mathrm{d}t \\ &\qquad{}-\int_{T}^{T+1}\int_{\Omega}\psi\rho u^{i}u^{j}\partial_{x_{j}}{\mathcal {B}}_{i} \biggl\{ S_{\epsilon}\bigl[b(\rho)\bigr]-\frac{1}{|\Omega|} \int_{\Omega}S_{\epsilon}\bigl[b(\rho)\bigr]\,\mathrm{d}x \biggr\} \,\mathrm{d}x\,\mathrm{d}t \\ &\qquad{}+\int_{T}^{T+1}\int_{\Omega}\psi\rho u^{i} {\mathcal {B}}_{i} \biggl\{ S_{\epsilon}\bigl[\bigl(b(\rho)-b'(\rho)\rho\bigr)\operatorname{div} {\mathbf{u}} \bigr] \\ &\qquad{}-\frac{1}{|\Omega|}\int_{\Omega}S_{\epsilon}\bigl[ \bigl( b(\rho)-b'(\rho)\rho\bigr)\operatorname{div} {\mathbf{u}} \bigr]\,\mathrm{d}x \biggr\} \,\mathrm{d}x\,\mathrm{d}t \\ &\qquad{}+ \int_{T}^{T+1}\int_{\Omega}\psi\rho u^{i} {\mathcal {B}}_{i} \biggl\{ r_{\epsilon}- \frac{1}{|\Omega|}\int_{\Omega}r_{\epsilon}\,\mathrm{d}x \biggr\} \,\mathrm{d}x\,\mathrm{d}t \\ &\qquad{}- \int_{T}^{T+1}\int_{\Omega}\psi\rho u^{i} {\mathcal {B}}_{i} \bigl\{ \operatorname{div} \bigl(S_{\epsilon}\bigl[b(\rho)\bigr]\bigr){\mathbf{u}} \bigr\} \,\mathrm{d}x \,\mathrm{d}t \\ &\qquad{}-\int_{T}^{T+1}\int_{\Omega}\psi\rho f_{i} {\mathcal {B}}_{i} \biggl\{ S_{\epsilon}\bigl[b(\rho)\bigr]-\frac{1}{|\Omega|}\int_{\Omega}S_{\epsilon}\bigl[b(\rho)\bigr]\,\mathrm{d}x \biggr\} \,\mathrm{d}x\,\mathrm{d}t . \end{aligned}$$
(47)
Using the condition (38), we can get the following estimates; please, refer to [2] for the omitted details:
$$\begin{aligned}& \biggl| \int_{T}^{T+1}\psi \biggl(\int _{\Omega}a\rho^{5/3} \,\mathrm{d}x \biggr) \biggl( \frac{1}{|\Omega|}\int_{\Omega}S_{\varepsilon}\bigl[b(\rho) \bigr] \,\mathrm{d}x \biggr)\,\mathrm{d}t \biggr|\leq c_{5} \int _{T}^{T+1}\int_{\Omega}\rho^{5/3} \,\mathrm{d}x\,\mathrm{d}t, \end{aligned}$$
(48)
$$\begin{aligned}& \biggl|\int_{T}^{T+1}\int_{\Omega}\psi S_{\varepsilon}\bigl[b(\rho)\bigr] \operatorname{div} {\mathbf{u}}\,\mathrm{d}x \,\mathrm{d}t \biggr|\leq c_{6} \int_{T}^{T+1}\bigl\| { \mathbf{u}}(t)\bigr\| _{W_{0}^{1,2}(\Omega)}\,\mathrm{d}t, \end{aligned}$$
(49)
$$\begin{aligned}& \begin{aligned}[b] &\biggl|\int_{T}^{T+1}\int_{\Omega}\psi _{t}\rho u^{i}{\mathcal {B}}_{i} \biggl\{ S_{\varepsilon}\bigl[b(\rho)\bigr]-\frac{1}{|\Omega|}\int_{\Omega}S_{\varepsilon}\bigl[b(\rho)\bigr] \,\mathrm{d}x \biggr\} \,\mathrm{d}x\,\mathrm{d}t \biggr|\\ &\quad\leq c_{7} \int_{T}^{T+1}| \psi_{t}|\|\sqrt{\rho} {\mathbf{u}}\|_{L^{2}(\Omega)} \,\mathrm{d}t, \end{aligned} \end{aligned}$$
(50)
$$\begin{aligned}& \begin{aligned}[b] & \biggl|\int_{T}^{T+1}\int _{\Omega}\psi\partial_{x_{j}} u^{i} \partial_{x_{j}}{\mathcal {B}}_{i} \biggl\{ S_{\varepsilon}\bigl[b(\rho)\bigr]-\frac{1}{|\Omega|}\int_{\Omega}S_{\varepsilon}\bigl[b(\rho)\bigr] \,\mathrm{d}x \biggr\} \,\mathrm{d}x\,\mathrm{d}t \biggr| \\ &\quad\leq c_{8} \int_{T}^{T+1}\bigl\| { \mathbf{u}}(t)\bigr\| _{W_{0}^{1,2}(\Omega)}\,\mathrm{d}t, \end{aligned} \end{aligned}$$
(51)
$$\begin{aligned}& \begin{aligned}[b] & \biggl|\int_{T}^{T+1} \int_{\Omega}\psi\rho u^{i}u^{j} \partial_{x_{j}}{\mathcal {B}}_{i} \biggl\{ S_{\varepsilon}\bigl[b(\rho)\bigr]-\frac{1}{|\Omega|}\int_{\Omega}S_{\varepsilon}\bigl[b(\rho\bigr] \,\mathrm{d}x \biggr\} \,\mathrm{d}x\,\mathrm{d}t \biggr| \\ &\quad\leq c_{9} \sup_{t\in[T,T+1]}\bigl\| \rho(t) \bigr\| _{L^{5/3}(\Omega)}\int_{T}^{T+1}\bigl\| {\mathbf{u}}(t) \bigr\| _{W_{0}^{1,2}(\Omega)}^{2}\,\mathrm{d}t, \end{aligned} \end{aligned}$$
(52)
$$\begin{aligned}& \begin{aligned}[b] & \biggl|\int_{T}^{T+1}\int _{\Omega}\psi\rho u^{i}\mathcal {B}_{i} \biggl\{ S_{\varepsilon}\bigl[\bigl(b(\rho)-b'(\rho)\rho\bigr) \operatorname{div} {\mathbf{u}} \bigr] \\ &\qquad{}-\frac{1}{|\Omega|}\int_{\Omega}S_{\varepsilon}\bigl[(b(\rho)-b'(\rho)\rho\operatorname{div} {\mathbf{u}} \bigr] \,\mathrm{d}x \biggr\} \,\mathrm{d}x\,\mathrm{d}t \biggr| \\ &\quad\leq c_{10} \sup_{t\in[T,T+1]}\bigl\| \rho(t) \bigr\| _{L^{5/3}(\Omega)}\int_{T}^{T+1}\bigl\| {\mathbf{u}}(t) \bigr\| _{W_{0}^{1,2}(\Omega)}^{2}\,\mathrm{d}t, \end{aligned} \end{aligned}$$
(53)
$$\begin{aligned}& \begin{aligned}[b] & \biggl|\int_{T}^{T+1}\int _{\Omega}\psi\rho u^{i} {\mathcal {B}}_{i} \biggl\{ r_{\varepsilon}-\frac{1}{|\Omega|}\int r_{\varepsilon}\biggr\} \,\mathrm{d}x\,\mathrm{d}t \biggr| \\ &\quad\leq c_{11}\int_{T}^{T+1}\|\rho \|_{L^{5/3}(\Omega)} \|\mathbf{u}\|_{W^{1,2}(\Omega)}\|r_{\varepsilon}\|_{L^{5/3}(\Omega )}\,\mathrm{d}t, \end{aligned} \end{aligned}$$
(54)
$$\begin{aligned}& \begin{aligned}[b] & \biggl|\int_{T}^{T+1} \int_{\Omega}\psi\rho f_{i} {\mathcal {B}}_{i} \bigl\{ \operatorname{div} \bigl(S_{\varepsilon}\bigl[b(\rho) \bigr]\mathbf {u} \bigr) \bigr\} \,\mathrm{d}x \,\mathrm{d}t\biggr| \\ &\quad\leq c_{12} \sup_{t\in[T,T+1]}\bigl\| \rho(t) \bigr\| _{L^{5/3}(\Omega)}\int_{T}^{T+1}\bigl\| {\mathbf{u}}(t) \bigr\| _{W_{0}^{1,2}(\Omega)}^{2}\,\mathrm{d}t, \end{aligned} \end{aligned}$$
(55)
and
$$ \biggl|\int_{T}^{T+1}\int _{\Omega}\psi\rho f_{i}{\mathcal {B}}_{i} \biggl\{ S_{\varepsilon}\bigl[b(\rho)\bigr]-\frac{1}{|\Omega|}\int _{\Omega}S_{\varepsilon}\bigl[b(\rho)\bigr]\,\mathrm{d}x \biggr\} \,\mathrm{d}x\,\mathrm{d}t \biggr|\leq c_{13}(K ). $$
(56)
In addition, we can use (46) to see that
$$b(\rho)\mbox{ is in } L_{\mathrm{loc}}^{\infty}\bigl(R^{+}, L^{10}(\Omega)\bigr) , $$
thus, exploiting (42) and (54), we further get
$$ \lim_{\varepsilon\rightarrow 0+} \biggl|\int_{T}^{T+1} \int_{\Omega}\psi\rho u^{i} {\mathcal {B}}_{i} \biggl\{ r_{\varepsilon}-\frac{1}{|\Omega|}\int r_{\varepsilon}\biggr\} \,\mathrm{d}x\,\mathrm{d}t \biggr|=0. $$
(57)
Noting that there exists a sequence \(\psi_{\varepsilon}\) approximating the characteristic function of the interval \([T, T+1]\), thus, letting \(\varepsilon\rightarrow0\) in (48)-(56), we can obtain
$$ \begin{aligned}[b] \int_{T}^{T+1} \int _{\Omega}\rho^{26/15}\,\mathrm{d}x\,\mathrm{d}t \leq{}&c_{15}(K ) \biggl[1+ \sup_{t\in[T,T+1]}\bigl\| \sqrt{\rho} { \mathbf{u}}(t)\bigr\| _{L^{2}(\Omega)}\\ &{}+\Bigl(1+\sup_{t\in[T,T+1]}\bigl\| \rho(t)\bigr\| _{L^{5/3}(\Omega)}\Bigr)\int _{T}^{T+1} \bigl\| {\mathbf{u}}(t)\bigr\| _{W_{0}^{1,2}(\Omega)}^{2} \,\mathrm{d}t \biggr]. \end{aligned} $$
(58)
Recalling the interpolating the spaces \(L^{1}\) and \(L^{26/15}\), we have
$$ \int_{T}^{T+1}\|\rho \|_{L^{5/3}(\Omega )}^{5/3} \,\mathrm{d}t\leq c_{16} m^{3/55} \biggl[\int_{T}^{T+1}\int _{\Omega}\rho^{26/15}\,\mathrm {d}x\,\mathrm{d}t \biggr]^{10/11}. $$
(59)
Then, exploiting Lemma 2.1, one has
$$\begin{aligned} & \biggl| \sup_{t\in[T,T+1]}\bigl\| \rho(t)\bigr\| _{L^{5/3}(\Omega )}\int _{T}^{T+1}\bigl\| {\mathbf{u}}(t)\bigr\| _{W_{0}^{1,2}(\Omega)}^{2} \,\mathrm{d}t \biggr|^{\frac{10}{11}} \\ &\quad\leq c_{17}(K ) \Bigl[1+ \sup_{t\in[T,T+1]}\bigl\| \rho(t) \bigr\| _{L^{5/3}(\Omega)} \sup_{t\in[T,T+1]} \bigl\| \rho(t)\bigr\| _{L^{\frac{3}{2}}(\Omega)} \Bigr]^{\frac{10}{11}} \\ &\quad\leq c_{18}(K ) \Bigl[1+\sup_{t\in[T,T+1]}\bigl\| \rho(t) \bigr\| _{L^{5/3}(\Omega)} \Bigr]^{5/3}. \end{aligned}$$
(60)
In addition, thanks to (5), we have
$$ \operatorname{ess}\sup_{t\in[T,T+1]}\bigl\| \sqrt{\rho} { \mathbf{u}}(t)\bigr\| _{L^{2}(\Omega)}\leq \sup_{t\in[T,T+1]}2\sqrt{E(t+)}. $$
(61)
Finally, making use of Lemma 2.2 and the estimates (58)-(61), we conclude
$$\begin{aligned} &\sup_{t\in[T,T+1]}E(t+) \\ &\quad\leq c_{19}(K ) \Bigl(1+\sup_{t\in[T,T+1]}2 \sqrt{E(t+)}+m^{3/55} \sup_{t\in[T,T+1]}\bigl\| \rho(t) \bigr\| _{L^{5/3}(\Omega)} ^{5/3} \Bigr). \end{aligned}$$
(62)
Consequently, (62) implies the existence of the constant L which has the property stated in Proposition 2.2 provided that
$$m\leq\min \biggl\{ \biggl(\frac{a}{2c_{19}(K)(\gamma-1)} \biggr)^{\frac {55}{3}},m_{0} \biggr\} . $$
This completes the proof of Proposition 2.2.

Declarations

Acknowledgements

The authors appreciate the anonymous referees for useful comments and suggestions on our manuscript, which improved the presentation of this article. The research of Xiaoying Wang was supported by NSFC (U1430103), Beijing Higher Education Young Elite Teacher Project (YETP0724) and the Fundamental Research Funds for the Central Universities (13MS35), and Weiwei Wang was supported by NSFC (11501116).

Open Access This article is distributed under the terms of the Creative Commons Attribution 4.0 International License (http://creativecommons.org/licenses/by/4.0/), which permits unrestricted use, distribution, and reproduction in any medium, provided you give appropriate credit to the original author(s) and the source, provide a link to the Creative Commons license, and indicate if changes were made.

Authors’ Affiliations

(1)
School of Mathematics and Physics, North China Electric Power University
(2)
College of Mathematics and Computer Science, Fuzhou University

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