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Solutions for the quasi-linear elliptic problems involving the critical Sobolev exponent
Journal of Inequalities and Applications volume 2017, Article number: 217 (2017)
Abstract
In this article, we study the existence and multiplicity of positive solutions for the quasi-linear elliptic problems involving critical Sobolev exponent and a Hardy term. The main tools adopted in our proofs are the concentration compactness principle and Nehari manifold.
1 Introduction
In this article, we consider the following quasi-linear elliptic problem:
where \(\Omega\subset\mathbb{R}^{N}\ (N\geq3)\) is a bounded domain with the smooth boundary ∂Ω such that \(0\in\Omega\). \(\Delta _{p}u=\operatorname{div}( \vert \nabla u \vert ^{p-2}\nabla u)\) is the p-Laplacian operator of u, \(1< p< N, \lambda>0\) is a positive real number. \(0\leq\mu<\overline {\mu}\) (\(\overline{\mu}=\frac{(N-p)^{p}}{p}\) is the best Hardy constant). \(1< q< p\) and \(p^{*}=\frac{Np}{N-p}\) is the critical Sobolev exponent. \(0<\alpha<p-1\), \(0<\beta<\beta_{1}\) (\(\beta_{1}\) is the first eigenvalue that \(-\Delta_{p}u-\mu\frac{ \vert u \vert ^{p-2}u}{ \vert x \vert ^{p}}= \vert x \vert ^{\alpha -p} \vert u \vert ^{p-2}u\) under Dirichlet boundary condition).
Definition 1.1
The function \(u\in W_{0}^{1,p}(\Omega)\) is called a weak solution of (1.1) if u satisfies
for all \(v\in W_{0}^{1,p}(\Omega)\).
In this paper, we use the following norm of \(W_{0}^{1,p}(\Omega)\):
By the Hardy inequality (see [1, 2])
so this norm is equivalent to \((\int_{\Omega} \vert \nabla u \vert ^{p}\,dx)^{\frac {1}{p}}\), the usual norm in \(W_{0}^{1,p}(\Omega)\).
The norm in \(L^{p}(\Omega)\) is represented by \(\Vert u \Vert _{p}=(\int_{\Omega } \vert u \vert ^{p}\,dx)^{\frac{1}{p}}\). According to Hardy inequality, the following best Sobolev constant is well defined for \(1< p< N\), and \(0\leq\mu<\overline{\mu}\):
The quasi-linear problems on Hardy inequality have been studied extensively, either in the smooth bounded domain or in the whole space \(\mathbb{R}^{N}\). More and more excellent results have been obtained, which provide us opportunities to understand the singular problems. However, compared with the semilinear case, the quasi-linear problems related to Hardy inequality are more complicated [3–16]. Abdellaoui, Felli and Peral [3] considered the extremal function which achieves the best constant \(S_{\mu,0}\), and gave the properties of the extremal functions. The conclusions obtained in [3] can be applied in the problems with critical Sobolev exponent and Hardy term.
Wang, Wei and Kang [10] investigated the following problem:
where \(1< q< p, \mu>0\), f and g are non-negative functions and \(p^{*}=\frac{Np}{N-p}\) is the critical Sobolev exponent. The property of the Nehari manifold was used to prove the existence of multiple positive solutions for (1.4). Furthermore, Hsu [11, 12] improved and complemented the main results obtained in [10]. Recently, Goyal and Sreenadh [13] investigated a class of singular N-Laplacian problems with exponential nonlinearities in \(\mathbb{R}^{N}\). Very recently, Xiang [14] established the asymptotic estimates of weak solutions for p-Laplacian equation with Hardy term and critical Sobolev exponent.
We should mention that Liu, Guo and Lei [17] studied the existence and multiplicity of positive solutions of Kirchhoff equation with critical exponential nonlinearity. Inspired by [17, 18], we study the problem (1.1) on critical Sobolev exponent. Comparing with the main results obtained in [4, 6, 10–12], in this paper, on the one hand, we will analysis the effect of \(\beta \vert x \vert ^{\alpha-p} \vert u \vert ^{p-2}u\), and the more careful estimates are needed. On the other hand, we establish an lower bound for \(\lambda_{*}\) (\(\lambda_{*}\) is defined in Theorem 1.1).
Define the energy functional associated to problem (1.1) as follows:
We obtain the following result.
Theorem 1.1
Suppose that \(1< q< p\), \(0<\alpha <p-1\). Then there exists \(\lambda_{*}>0\) such that problem (1.1) admits at least two solutions and one of the solutions is a ground state solution for all \(\lambda\in(0,\lambda_{*})\).
2 Preliminaries
Firstly, we introduce the Nehari manifold
Furthermore \(u\in\mathcal{N}_{\lambda}\) if and only if
Let
then
\(\mathcal{N}_{\lambda}\) can be divided into the following three parts:
Applying the Hölder inequality and the Sobolev inequality, for all \(u\in W_{0}^{1,p}(\Omega)\backslash\{0\}\) we have
Lemma 2.1
Assume that \(\lambda\in(0,T_{1})\) with
Then (i) \(\mathcal{N}_{\lambda}^{\pm}\neq\emptyset\), and (ii) \(\mathcal {N}_{\lambda}^{0}=\emptyset\).
Proof
(i) We define a function \(\Phi\in C(\mathbb {R}^{+},\mathbb{R})\) by
Let \(\Phi^{\prime}(s)=0\), that is,
We can deduce that
It is easy to check that \(\Phi^{\prime}(s)>0\) for all \(0< s< s_{\max}\) and \(\Phi^{\prime}(s)<0\) for all \(s>s_{\max}\). Consequently, \(\Phi(s)\) attains its maximum at \(s_{\max}\), that is,
Since
where \(0<\lambda<T_{1}\). Thus, there exist constants \(s^{+}\) and \(s^{-}\) such that
(ii) We prove that \(\mathcal{N}_{\lambda}^{0}=\emptyset\) for all \(\lambda\in(0,T_{1})\). By contradiction, assume that there exists \(u_{0}\neq 0\) such that \(u_{0}\in\mathcal{N}_{\lambda}^{0}\). From (2.1), we have
combining with (2.3), we obtain
Equations (2.6) and (2.7) imply that
that is,
Similarly,
that is,
Note that (1.3) holds for \(u\in\mathcal{N}_{\lambda}^{0}\backslash\{0\} \). Then
It follows from (2.8) and (2.9) that
for \(0<\lambda<T_{1}\). This is a contradiction. □
Lemma 2.2
\(I_{\lambda}\) is coercive and bounded below on \(\mathcal{N}_{\lambda}\).
Proof
For \(u\in\mathcal{N}_{\lambda}\), we can deduce from (1.3) and (2.5) that
Note that \(1< q< p\) and \(0<\beta<\beta_{1}\), we see that \(I_{\lambda}\) is coercive and bounded below on \(\mathcal{N}_{\lambda}\). □
From Lemma 2.1, we know that \(\mathcal{N}_{\lambda}^{+}\) and \(\mathcal {N}_{\lambda}^{-}\) are nonempty. Furthermore, taking into account Lemma 2.2, we define
Lemma 2.3
\(\kappa_{\lambda}\leq\kappa_{\lambda}^{+}<0\).
Proof
For \(u\in\mathcal{N}_{{\lambda}}^{+}\), using (2.1) and (2.2), we have
and
that is,
By (2.10), we get
Therefore, we have \(\kappa_{\lambda}\leq\kappa_{\lambda}^{+}<0\). □
Lemma 2.4
For \(u\in\mathcal{N}_{\lambda}\), there exist \(\varepsilon>0\) and a differentiable function \(\widehat {f}=\widehat{f}(\omega): B(0,\varepsilon)\subset W_{0}^{1,p}(\Omega )\longrightarrow\mathbb{R}^{+}\) such that
Proof
Define
as follows:
It is clear that
and
which implies that
Lemma 2.1 tells us that \(\widehat{F}_{s}(1,0)\neq0\). Thus, by the implicit function theorem at the point \((0,1)\), there exist \(\varepsilon >0\), and a differentiable function
such that
 □
Lemma 2.5
For \(u\in\mathcal{N}_{\lambda}^{-}\), there exist \(\varepsilon>0\) and a differentiable function \(\widetilde {f}=\widetilde{f}(v): B(0,\varepsilon)\subset W_{0}^{1,p}(\Omega )\longrightarrow\mathbb{R}^{+}\) such that
Proof
The proof is similar to that of Lemma 2.4, and we omit it here. □
Lemma 2.6
If \(\{u_{n}\}\subset\mathcal {N}_{\lambda}\) is a minimizing sequence of \(I_{\lambda}\), for every \(\phi \in W_{0}^{1,p}(\Omega)\), then
Proof
It follows from Lemma 2.2 that \(I_{\lambda}\) is coercive on \(\mathcal{N}_{\lambda}\). Using the Ekeland variational principle [19], we can find a minimizing sequence \(\{u_{n}\}\subset \mathcal{N}_{\lambda}\) of \(I_{\lambda}\) satisfying
Without loss of generality, we can assume that \(u_{n}\geq0\). By Lemma 2.2, we know that \(\{u_{n}\}\) is bounded in \(W_{0}^{1,p}(\Omega)\). As a consequence, there exist a subsequence (still denoted by \(\{u_{n}\}\)) and \(u_{*}\) in \(W_{0}^{1,p}(\Omega)\) such that
From Lemma 2.4, for \(s>0\) sufficiently small and \(\phi\in W_{0}^{1,p}(\Omega)\), and set \(u=u_{n}\), \(\omega=s\phi\in W_{0}^{1,p}(\Omega)\), we can find that \(f_{n}(s)=f_{n}(s\phi)\) such that \(f_{n}(0)=1\) and \(f_{n}(s)(u_{n}+s\phi)\in\mathcal{N}_{\lambda}\). Since
By (2.12), we obtain
Notice that
Therefore
Dividing by \(s>0\) and taking the limit for \(s\rightarrow0\), combining with (2.14) and (2.15), we have
Consequently
for every \(\phi\in W_{0}^{1,p}(\Omega)\). Note that (2.16) holds equally for −ϕ, we see that (2.11) holds. □
Lemma 2.7
Set \(D^{1,p}(\mathbb {R}^{N})=\{u\in L^{p^{*}}(\mathbb{R}^{N}): \vert \nabla u \vert \in L^{p} (\mathbb{R}^{N})\}\). Assume that \(1< p< N\) and \(0\leq\mu<\overline{\mu}\). Then the limiting problem
has radially symmetric ground states
such that
where the function \(U_{p,\mu}(x)=U_{p,\mu}( \vert x \vert )\) is the unique radial solution of the above limiting problem with
In the following, we define \(\Lambda=\frac{1}{N}S_{\mu,0}^{\frac{N}{p}}\).
Lemma 2.8
Let \(\{u_{n}\}\subset\mathcal {N}^{-}_{\lambda}\) be a minimizing sequence for \(I_{\lambda}\) with \(\kappa_{\lambda}^{-}<\Lambda-D\lambda^{\frac{p}{p-q}}\), where
Then there exists \(u\in W_{0}^{1,p}(\Omega)\) such that \(u_{n}\rightarrow u\) in \(L^{p^{*}}(\Omega)\).
Proof
Since
By Lemma 2.2, we know that \(\{u_{n}\}\) is bounded in \(W_{0}^{1,p}(\Omega )\). In fact, we can deduce from (1.3) and (2.19) that
where \(0<\beta<\beta_{1}\), \(1< q< p\), we see that \(\{u_{n}\}\) is bounded in \(W_{0}^{1,p}(\Omega)\). We can choose a subsequence (still denoted by \(\{u_{n}\}\)) and \(u\in W_{0}^{1,p}(\Omega)\) satisfying
In term of the concentration compactness principle, going if necessary to a subsequence, there exist an at most countable set \(\mathcal{J}\), a set of points \(\{x_{j}\}_{j\in\mathcal{J}}\subset\Omega\setminus\{0\} \), and real numbers \(\mu_{j}\), \(\nu_{j}\), \(\widetilde{\chi_{0}}\) such that
where \(\delta_{x_{j}}\) is the Dirac mass at \(x_{j}\).
Let ϵ be sufficient small satisfying \(0\notin B(x_{j}, \epsilon )\) and \(B(x_{j}, \epsilon)\cap B(x_{i}, \epsilon)=\emptyset\) for \(i\neq j, i, j=1, 2, \ldots, k\). Let \(\psi_{\epsilon,j}(x)\) be a smooth cut-off function centered at \(x_{j}\) such that \(0\leq\psi_{\epsilon ,j}(x)\leq1\), \(\psi_{\epsilon,j}(x)=1\) for \(x\in B(x_{j}, \frac{\epsilon}{2})\), \(\psi_{\epsilon,j}(x)=0\) for \(x\in\Omega\backslash B(x_{j},\epsilon)\) and \(\vert \nabla\psi_{\epsilon,j}(x) \vert \leq\frac{4}{\epsilon}\). Note that
Furthermore, we have
By (1.3), we deduce that
and
Since \(\{u_{n}\}\) is bounded in \(W_{0}^{1,p}(\Omega)\), and \(u_{n}\rightharpoonup u\) weakly in \(L^{p^{*}}(\Omega)\), we conclude that
and
By (2.11), we have
Since \(S_{0,0}\nu_{j}^{\frac{p}{p^{*}}}\leq\mu_{j}\), we have \(\mu_{j}=\nu _{j}=0\) or \(\mu_{j}\geq(S_{0,0})^{\frac{N}{p}}\).
On the other hand, let \(\epsilon>0\) be sufficiently small satisfying \(x_{j}\notin B(0, \epsilon)\), \(\forall j\in\mathcal{J}\). Let \(\psi _{\epsilon,0}(x)\) a smooth cut-off function centered at the origin such that \(0\leq\psi_{\epsilon,0}(x)\leq1\), \(\psi_{\epsilon,0}(x)=1\) for \(\vert x \vert \leq\frac{\epsilon}{2}\), \(\psi_{\epsilon,0}(x)=0\) for \(\vert x \vert \geq \epsilon\) and \(\vert \nabla\psi_{\epsilon,0}(x) \vert \leq\frac{4}{\epsilon}\). Hence, we have
and
Therefore
Combining the definition of \(S_{\mu,0}\), we get that \(S_{\mu,0}\nu _{0}^{\frac{p}{p^{*}}}\leq\mu_{0}-\mu\widetilde{\chi_{0}}\leq\nu_{0}\), which implies that \(\nu_{0}=0\) or \(\nu_{0}\geq(S_{\mu,0})^{\frac {N}{p}}\). Now, we prove that \(\mu_{j}\geq(S_{0,0})^{\frac{N}{p}}\) and \(\nu_{0}\geq(S_{\mu,0})^{\frac{N}{p}}\) are not true. If not, we have
where D is defined in (2.18). Hence, we conclude that \(\Lambda-D\lambda^{\frac{p}{p-q}}\leq\kappa _{\lambda}^{-}<\Lambda-D\lambda^{\frac{p}{p-q}}\), which is a contradiction. It follows that \(\nu_{j}=0\) for \(j\in\{0\}\cup\mathcal{J}\), which means that \(\int_{\Omega} \vert u_{n} \vert ^{p^{*}}\,dx\rightarrow\int_{\Omega } \vert u \vert ^{p^{*}}\,dx\) as \(n\rightarrow\infty\). The proof is completed. □
In the following, we need some estimates for the extremal function \(V_{\epsilon}\) defined in Lemma 2.7. Given \(R>0\), let \(\varphi(x)\in W_{0}^{1,p}(\Omega)\), \(0\leq\varphi(x)\leq1\), \(\varphi(x)=1\) for \(\vert x \vert \leq R\), \(\varphi(x)=0\) for \(\vert x \vert \geq2R\). Set \(v_{\epsilon }(x)=\varphi(x)V_{\epsilon}(x)\). For \(1< p< N\) and \(1< q< p^{*}\), we have the following estimates (see [4, 6]):
then
where \(b(\mu)\) is the zero of the function
satisfying \(0<\frac{N-p}{p}<b(\mu)<\frac{N-p}{p-1}\).
Lemma 2.9
There exists \(\lambda_{0}>0\) such that
where Λ and D are defined in Lemma 2.8.
Proof
For two positive constants \(s_{0}\) and \(s_{1}\) (independent of ϵ, λ), we show that there exists \(s_{\epsilon}>0\) with \(0< s_{0}\leq s_{\epsilon}\leq s_{1}<\infty\) such that \(\sup_{s\geq0}I_{\lambda}(sv_{\epsilon})=I_{\lambda }(s_{\epsilon}v_{\epsilon})\). In fact, since \(\lim_{s\rightarrow+\infty}I_{\lambda}(sv_{\epsilon })=-\infty\), we can deduce that
and
Equations (2.24) and (2.25) imply that
That is,
Hence, we can obtain from (2.26) that \(s_{\epsilon}\) is bounded below. Moreover, it is clear to see from (2.24) that \(s_{\epsilon}\) is bounded above for all \(\epsilon>0\) small enough. Therefore, our claim holds.
Set
In the following, we prove that
Let
Direct computations give us that \(\lim_{s\rightarrow\infty}\widetilde {h}(s)=-\infty\) and \(\widetilde{h}(0)=0\). Thus \(\sup_{s\geq0}\widetilde{h}(s)\) is obtained at some \(S_{\epsilon }>0\), and
Since \(\widetilde{h}^{\prime}(s) \vert _{S_{\epsilon}}=0 \), that is,
It is easy to check that \(h(s)\) is increasing in \([0,S_{\epsilon})\), according to (2.21) and (2.22), we have
Therefore, by (2.27), we have
Now, we consider the following cases:
(i) \(\frac{N}{b(\mu)}< q< p\). Choose \(\epsilon=\lambda^{\frac{1}{(p-q)(b(\mu)-\frac{N}{p}+1)}}\), for \(\lambda<\lambda_{1}:=(\frac{C_{1}+D}{C_{2}})^{\frac{(p-q)(b(\mu)-\frac {N}{p}+1)}{N-qb(\mu)}}\), we have
(ii) \(q=\frac{N}{b(\mu)}\). We still choose \(\epsilon=\lambda^{\frac{1}{(p-q)(b(\mu)-\frac {N}{p}+1)}}\), for \(\lambda<\lambda_{2}:= e^{-(\frac{C_{1} +D}{C_{3}})}\), we have
where \(C_{3} =\frac{C_{2}}{(p-q)(b(\mu)-\frac{N}{p}+1)}\).
(iii) \(1< q<\frac{N}{b(\mu)}\). Put \(\epsilon^{p(b(\mu)-\frac {N}{p}+1)}\leq\lambda^{\frac{p}{p-q}}\), for \(\lambda<\lambda_{3}:=(\frac{C_{2} -D}{C_{1}})^{\frac{p-q}{pq-p}}\) with \(C_{2} >D\), we have
Consequently, for \(\lambda<\lambda_{0}:=\min\{\lambda_{1}, \lambda_{2}, \lambda_{3}\}\), we deduce that
 □
3 Proof of main result
We can find a constant \(\delta>0\) such that \(\Lambda-D\lambda^{\frac {p}{p-q}}>0\) for \(\lambda<\delta\). Let \(\lambda_{*}=\min\{T_{1}, \delta, \lambda_{0}\}\). For \(\lambda\in(0,\lambda_{*})\), Lemmas 2.1-2.4, 2.6 and 2.8 hold.
Let \(\{u_{n}\}\subset\mathcal{N}_{\lambda}\) be a minimizing sequence of \(I_{\lambda}\). It is easy to see that \(\{u_{n}\}\) is bounded in \(W_{0}^{1,p}(\Omega)\) and there exist a subsequence of \(\{u_{n}\}\) (still denoted by \(\{u_{n}\}\)) and \(u_{\lambda}\in W_{0}^{1,p}(\Omega)\) such that
as \(n\rightarrow\infty\).
Firstly, by Lemma 2.4, we can know that \(f_{n}^{\prime}(0)\) is bounded with respect to \(n\in\mathbb{N}\). Letting \(n\rightarrow\infty\) in (2.11), we deduce that
for all \(\phi\in W_{0}^{1,p}(\Omega)\). Equation (3.2) implies that \(u_{\lambda}\) is a solution of (1.1). We claim that \(u_{\lambda}\not\equiv0\). If not, \(u_{\lambda}=0\), since \(u_{n}\in\mathcal{N}_{\lambda}\), we have
Note that
Put \(\lim_{n\rightarrow\infty} \Vert u_{n} \Vert =m\), we conclude that \(m\geq S_{\mu,0}^{\frac{p^{*}}{p(p^{*} -p)}}\). By Lemma 2.8, we obtain
which contradicts with \(\kappa_{\lambda}<\Lambda-D\lambda^{\frac{p}{p-q}}\) (from Lemma 2.9).
Secondly, we prove that \(u_{\lambda}\in\mathcal{N}_{\lambda}^{+}\). Suppose that this is not true, \(i.e\)., \(u_{\lambda}\in\mathcal {N}_{\lambda}^{-}\). From Lemma 2.1, we can find positive numbers \(s^{+}\) and \(s^{-}\) with \(s^{+}< s_{\max}< s^{-}=1\) such that \(s^{+}u_{\lambda}\in \mathcal{N}_{\lambda}^{+}\), \(s^{-}u_{\lambda}\in\mathcal{N}_{\lambda }^{-}\) and
which is a contradiction. Hence \(u_{\lambda}\in\mathcal{N}_{\lambda}^{+}\). Furthermore, combining with Lemma 2.3, we can obtain
Therefore, we see that \(u_{\lambda}\) is a non-negative ground state solution of problem (1.1).
In the following, we prove that problem (1.1) has a second solution \(v_{\lambda}\) with \(v_{\lambda}\in\mathcal{N}_{\lambda}^{-}\). Since \(I_{\lambda}\) is coercive on \(\mathcal{N}_{\lambda}^{-}\), according to the Ekeland variational principle and Lemma 2.9, there exists a minimizing sequence \(\{v_{n}\}\subset\mathcal {N}_{\lambda}^{-}\) of \(I_{\lambda}\) such that
-
(i)
\(I_{\lambda}(v_{n})<\kappa_{\lambda}^{-}+\frac{1}{n}\);
-
(ii)
\(I_{\lambda}(u)\geq I_{\lambda}(v_{n})-\frac{1}{n} \Vert u-v_{n} \Vert \) for all \(u\in\mathcal{N}_{\lambda}^{-}\).
Note that \(\{v_{n}\}\) is bounded in \(W_{0}^{1,p}(\Omega)\), there exist a subsequence (still denoted by \(\{v_{n}\}\)) and \(v_{\lambda}\in W_{0}^{1,p}(\Omega)\) such that
as \(n\rightarrow\infty\).
Similar to the above discussion, we can deduce that \(v_{n}\rightarrow v_{\lambda}\) in \(W_{0}^{1,p}(\Omega)\) and \(v_{\lambda}\) is a non-negative solution of (1.1). Thirdly, we show that \(v_{\lambda}\neq0\) in Ω. According to \(v_{n}\in\mathcal{N}_{\lambda}^{-}\), we obtain
hence
together with \(v_{n}\rightarrow v_{\lambda}\) in \(W_{0}^{1,p}(\Omega)\) means that \(v_{\lambda}\not\equiv0\).
Lastly, we show that \(v_{\lambda}\in\mathcal{N}_{\lambda}^{-}\). We only need to prove that \(\mathcal{N}_{\lambda}^{-}\) is closed. In fact, for \(\{v_{n}\}\subset\mathcal{N}_{\lambda}^{-}\), it follows from Lemmas 2.8 and 2.9 that
In addition
Thus
which means that \(v_{\lambda}\in\mathcal{N}_{\lambda}^{0}\cup\mathcal {N}_{\lambda}^{-}\). Combining with Lemma 2.1 and \(v_{\lambda}\not\equiv0\), we see that \(\mathcal{N}_{\lambda}^{-}\) is closed. Note that \(\mathcal{N}_{\lambda}^{+}\cap\mathcal{N}_{\lambda }^{-}=\emptyset\), we know that \(u_{\lambda}\) and \(v_{\lambda}\) are different.
4 Conclusions
In this paper, we study the existence and multiplicity of positive solutions for the quasi-linear elliptic problem which consists of critical Sobolev exponent and a Hardy term.
The main conclusions of this work:
-
(1)
Adding a linear perturbation in the nonlinear term of elliptic equation.
-
(2)
The main challenge of this study is the lack of compactness of the embedding \(W_{0}^{1,p}\hookrightarrow L^{p^{*}}\). We overcome it by the concentration compactness principle.
-
(3)
We apply the Ekeland variational principle to obtain a minimizing sequence with good properties.
5 Discussion
In the future, a natural question is whether the multiplicity of positive solutions for (1.1) can be established with negative exponent \(\frac{1}{u^{\gamma}}\ (0<\gamma<1)\).
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Acknowledgements
This project is supported by the Natural Science Foundation of Shanxi Province (2016011003), Science Foundation of North University of China (110246), NSFC (11401583) and the Fundamental Research Funds for the Central Universities (16CX02051A).
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Sang, Y., Guo, S. Solutions for the quasi-linear elliptic problems involving the critical Sobolev exponent. J Inequal Appl 2017, 217 (2017). https://doi.org/10.1186/s13660-017-1492-y
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DOI: https://doi.org/10.1186/s13660-017-1492-y