\documentclass[reqno]{amsart}
\usepackage{hyperref}

\AtBeginDocument{{\noindent\small
\emph{Electronic Journal of Differential Equations},
Vol. 2015 (2015), No. 215, pp. 1--7.\newline
ISSN: 1072-6691. URL: http://ejde.math.txstate.edu or http://ejde.math.unt.edu
\newline ftp ejde.math.txstate.edu}
\thanks{\copyright 2015 Texas State University - San Marcos.}
\vspace{9mm}}

\begin{document}
\title[\hfilneg EJDE-2015/215\hfil Multiple solutions]
{Multiple solutions for Kirchhoff type problem near resonance}

\author[S.-Z. Song, C.-L. Tang,  S.-J. Chen \hfil EJDE-2015/215\hfilneg]
{Shu-Zhi Song, Chun-Lei Tang, Shang-Jie Chen}

\address{Shu-Zhi Song \newline
School of Mathematics and Statistics,
 Southwest University, Chongqing 400715, China}
\email{sjrdj@163.com}

\address{Chun-Lei Tang (corresponding author)\newline
School of Mathematics and Statistics,
Southwest University, Chongqing 400715,  China}
\email{tangcl@swu.edu.cn, Tel +8613883159865}

\address{Shang-Jie Chen \newline
School of Mathematics and Statistics, Chongqing
Technology and Business  University, Chongqing 400067, China}
\email{chensj@ctbu.edu.cn, 11183356@qq.com}

\thanks{Submitted March 23, 2015. Published August 17, 2015.}
\subjclass[2010]{35J61, 35C06, 35J20}
\keywords{Near resonance; mountain pass theorem; Kirchhoff type;
\hfill\break\indent Ekeland's variational principle}

\begin{abstract}
 Based on Ekeland's variational principle and the mountain pass theorem,
 we show the existence of three solutions to the  Kirchhoff type problem
 \begin{gather*}
 -\Big(a+b\int_{\Omega}|\nabla u|^2dx \Big) \Delta u
 =b \mu u^3+f(x,u)+h(x), \quad\text{in } \Omega, \\
 u=0,  \quad  \text{on } \partial \Omega.
 \end{gather*}
 Where the parameter $\mu$ is sufficiently close,
 from the left, to the first nonlinear eigenvalue.
\end{abstract}

\maketitle
\numberwithin{equation}{section}
\newtheorem{theorem}{Theorem}[section]
\newtheorem{lemma}[theorem]{Lemma}
\allowdisplaybreaks

\section{Introduction and statement of main result}

The articles shows the existence of multiple solutions for the Kirchhoff 
type problem with Dirichlet boundary condition,
\begin{equation}\label{problem1}
\begin{gathered}
-\Big(a+b\int_{\Omega}|\nabla u|^2dx \Big) \Delta u
 =b \mu u^3+f(x,u)+h(x), \quad \text{in }  \Omega, \\
 u=0, \quad \text{on } \partial \Omega,
 \end{gathered}
 \end{equation}
 where $\Omega$ is a bounded domain in $\mathbb{R}^N$ ($N=1,2,3$) with a smooth
 boundary $\partial \Omega$, $a\geq 0$, $b>0$ are real constants and $\mu$ 
 is a nonnegative parameter. Assume that $f\in C(\bar{\Omega} \times
\mathbb{R}, \mathbb{R})$ satisfies the sublinear growth condition:
\begin{itemize}
\item[(F1)]
$ \lim_{|t|\to  \infty}\frac{f(x,t)}{bt^3}=0$, uniformly for $x\in \Omega$.
\end{itemize}


Problem \eqref{problem1} can be looked on as a perturbed problem which was 
first studied by Mawhin and Schmit\cite{MS}, related to the two-point boundary 
value equation
\begin{equation} \label{15}
-u''-\lambda u =f(x,u)+h, \quad   u(0)=u(\pi)=0.
\end{equation}
Specifically, on the assumption: $\lambda<\lambda_1$ is sufficiently near 
to $\lambda_1$ ($\lambda_1$ is the first eigenvalue of the corresponding 
linear problem) and $f$ is bounded and satisfies a sign condition,  
the existence of three solutions to equation \eqref{15} was proved in \cite{MS}. 
Later, various papers related to the result appeared. We mention for example, 
\cite{ALS,MRS,MRS2,MP,OT}.  
 Ma, Ramos and Sanchez \cite{MRS} considered the boundary-value problem for
 $$
\Delta u+\lambda u + f(x,u)=h(x)
$$
defined on a bounded open set $\Omega \subset \mathbb{R}^N$. 
As the parameter $\lambda$ is sufficiently close to $\lambda_1$ 
from the left, there exist three solutions on both Dirchlet boundary 
conditions and Neumann boundary conditions. In addition, similar to the results 
in the linear case, the existence of three solutions was proved to the 
perturbed $p$-Laplacian equation in a bounded domain. Further consideration 
to the perturbed $p$-Laplacian equation in a bounded domain can be 
found in \cite{MRS2}. As for extension to the the perturbed $p$-Laplacian 
equation in the whole space $\mathbb{R}^N$, we refer to \cite{MP}. 
These results were also extended to some elliptic systems with the Dirichlet 
boundary conditions, refer to \cite{OT}. More recently, the authors 
in \cite{ALS} extended these conclusions to  some degenerate quasilinear 
elliptic systems with the Dirichlet boundary conditions. 
By analogy to the results mentioned above, we expect that problem \eqref{problem1} 
has at least three solutions as the parameter $\mu<\mu_1$ is sufficiently 
close to $\mu_1$. Here $\mu_1$ is the first eigenvalue of the  eigenvalue 
problem
\begin{gather*}
-\|u\|^2\Delta u=\mu u^3, \quad \text{in }\Omega, \\
u=0,\quad \text{on }\partial \Omega.
\end{gather*}

Let $H=H_0^1(\Omega)$ be the Hilbert space equipped with the norm 
$\|u\|=(\int_{\Omega}|\nabla u|^2 dx)^{1/2}$ and
$\|u\|_{L^s}=(\int_{\Omega}|u|^s dx)^{\frac{1}{s}}$ denote the norm of
$L^s(\Omega)$.
As shown in \cite{PZ} and \cite{ZP}, the first nonlinear eigenvalue 
$\mu_1>0$ is simple and has a eigenfunction $\psi_1 >0$ with 
$\|\psi_1\|_{L^4}=1$. Specifically, $\mu_1$ can be characterized by
\begin{equation}\label{principal character}
\mu_1=\inf\big\{\|u\|^4:\ u\in H,\ \int_{\Omega} |u|^4dx=1\big\}.
\end{equation}

Now we are in a position to state our result.

\begin{theorem} \label{thm1}
Suppose $f$ satisfies {\rm (F1)} and the following conditions:
\begin{itemize}
\item[(F2)] 
\[
\lim_{|t|\to  \infty}\int_{\Omega}F(x,t\psi_1)
-\frac{a}{2}\sqrt{\mu_1}t^2=+\infty,\quad \text{uniformly for } x\in \Omega,
\]
where $F(x,t)=\int_0^t f(x,s)ds$.

\item[(H1)]  $h\in L^2(\Omega)$ and 
$\int_{\Omega} h(x)\psi_1(x)dx =0$.
\end{itemize}
Then \eqref{problem1} has at least three solutions if $\mu <\mu_1$ 
is sufficiently close to $\mu_1$.
\end{theorem}

Many authors have studied the Kirchhoff type equation in a bounded domain 
by applying variational methods. For example, they consider Kirchhoff type 
problem
\begin{equation}\label{21}
 \begin{gathered}
 -\Big(a+b\int_{\Omega}|\nabla u|^2dx \Big) \Delta u=g(x,u),\quad  
  \text{in }\Omega , \\
u=0,\quad  \text{on }  \partial \Omega,
 \end{gathered}
\end{equation}
assuming that
\begin{equation}\label{22}
 \lim_{|t|\to  \infty}\frac{4G(x,t)}{bt^4}=\mu, \quad 
\text{uniformly in } x \in \Omega
\end{equation}
where $G(x,t)=\int_{0}^{t} g(x,s) ds$. For the case 
$\mu<\mu_1$ in \eqref{22}, the Euler functional corresponding to \eqref{21} 
is coercive. For the case $\mu=\mu_1$ in \eqref{22}, that is, problem \eqref{21} 
is resonance at the first nonlinear eigenvalue $\mu_1$,
the Euler functional corresponding to \eqref{21} is still coercive, together 
with the assumption that  $\lim_{|t|\to  \infty}[g(x,t)t-4G(x,t)]=+\infty$. 
So, the existence of weak solution for equation \eqref{21} is obtained based 
on the Least Action Principle (refer to \cite{YZ,YZ2,ZP}). 
Furthermore, provided $g$ with some conditions at zero, positive solution 
was obtained based on the topological degree argument (refer to \cite{LLS}),
 multiple solutions are found by means of invariant sets of descent flow
 method (refer to \cite{YZ,ZP}), or the Local Linking Theorem 
(refer to \cite{YZ2}). 
Our result is different from the results in 
\cite{LLS,YZ,YZ2,ZP} since we deal with the perturbation problem near 
to $\mu_1$ and all hypotheses on $f$ are just at infinity.

\section{Proof of main result}

We begin with some standard facts upon the variational formulation of
 problem \eqref{problem1}.
Let $I_{\mu}:H\mapsto \mathbb{R}$ be the functional defined by
\[
I_{\mu}(u)=\frac{a}{2}\|u\|^2+\frac{b}{4}\|u\|^4
-\frac{b \mu}{4}\int_{\Omega}|u|^4dx-\int_{\Omega}F(x,u)dx-\int_{\Omega}hudx.
\]
Since $f$ satisfies the sublinear growth condition (F1), it is
not difficult to verify that $I_{\mu}\in C^1(H,\mathbb{R})$. 
Furthermore, finding weak solutions of \eqref{problem1} is equivalent 
to finding critical points of functional $I_{\mu}$ in $H$.

Since $\Omega$ is a bounded domain in $\mathbb{R}^N$ $(N=1,2,3)$, the
embedding $H\hookrightarrow L^s(\Omega)$ is continuous for 
$s\in [1,2^*]$, compact for $s\in [1,2^*)$, 
\[
2^*=\begin{cases}
\frac{2N}{N-2},&  N=3,\\
+\infty,&  N=1,2.
\end{cases}
\]
Hence, for $s\in [1,2^*]$, there exists $\tau_s>0$ such that
\begin{equation}\label{sobolev insert}
\|u\|_{L^s}\leq \tau_s \|u\|,\quad \forall u\in H.
\end{equation}

We will prove the result by using Ekeland's variational principle 
\cite[Theorem 4.1]{willem} and a mountain pass theorem \cite{pucci}.  
For the convenience of readers, we state the mountain pass theorem as follows.

\begin{theorem}[{\cite[Corollary 1]{pucci}}] \label{thm2}
Consider a real Banach space $X$ and a function 
$I \in C^1(X,\mathbb{R})$. If the $(PS)$ condition holds and if $I$ has 
two different local mininum points, then $I$ possesses a third 
critical point.
\end{theorem}

To prove our theorem, using critical point theory, we need the 
Palais-Smale compactness. 


\begin{lemma} \label{lem1} 
Assume that {\rm (F1)} holds. Then any bounded $(PS)$ sequence of $I_{\mu}$ 
has a convergent subsequence in $H$.
\end{lemma}

\begin{proof}
  Let $\{u_n\}\subset H$ be a bounded $(PS)$ sequence of $I_{\mu}$; that is,
\begin{equation}\label{bound ps}
\|u_n\|\leq c, \quad |I_{\mu}(u_n)|\leq c ,\quad \|I'_{\mu}(u_n)\|\to  0,
\end{equation}
where $c$ denotes positive constant.
By  the reflexivity of $H$, we can assume that there exists $u\in H$ such that
\begin{gather}\label{13}
u_n\rightharpoonup u \quad  \text{weakly in } H,\\
\label{11}
u_n \to  u\quad \text{strongly in } L^p(\Omega)\; (1\leq p<2^*).
\end{gather}
It follows from (F1) that for any $\varepsilon>0$, there exits 
$M_{\varepsilon}>0$ such that
\begin{equation}\label{9}
|f(x,t)|\leq b\varepsilon |t|^3 +M_{\varepsilon},\quad
 \forall (x,t)\in \Omega\times {\mathbb{R}}.
\end{equation}
We can now put together the results in 
\eqref{sobolev insert}, \eqref{bound ps}, \eqref{11} and \eqref{9} 
to conclude that
\begin{equation}\label{31}
\begin{aligned}
\big|\int_{\Omega}f(x,u_n)(u-u_n)dx\big|
&\leq \int_{\Omega}|f(x,u_n)||u-u_n|dx \\
&\leq \int_{\Omega}(b\varepsilon |u_n|^3 +M_{\varepsilon})|u-u_n|dx \\
&\leq b\varepsilon\|u_n\|_{L^4}^{3}\|u-u_n\|_{L^4}
 +M_{\varepsilon}|\Omega|^{1/2}\|u-u_n\|_{L^2} \\
&\leq b \tau_4^3\varepsilon \|u_n\|^{3}\|u-u_n\|_{L^4}
 + M_{\varepsilon}|\Omega|^{1/2}\|u-u_n\|_{L^2} \\
&\leq c (\|u-u_n\|_{L^4}+\|u-u_n\|_{L^2}) \to  0,\quad \text{ as }
 n\to  \infty,
\end{aligned}
\end{equation}
where $c=\max\{b \tau_4^3\varepsilon,M_{\varepsilon}|\Omega|^{1/2}\}$,
and $|\Omega|$ is the measure of $\Omega$.
Similarly, we may deduce that
\begin{equation}\label{32}
\int_{\Omega}(|u_n|^2u_n(u-u_n)-|u|^2u(u-u_n))dx\to  0,\quad \text{as }
 n\to  \infty.
\end{equation}
From \eqref{bound ps} and \eqref{11}, we have
$$
\langle I_{\mu}'(u_n)-I_{\mu}'(u),u-u_n\rangle \to  0,\quad  \text{as }
 n\to  \infty,
$$
which combining with $\eqref{31}, \eqref{32}$, implies
$\|u_n\|\to  \|u\|$  as $n\to  \infty$.
 It follows from \eqref{13} that $u_n\to  u$ in $H$.
\end{proof}

Set
$$
V=\big\{v\in H: \int_{\Omega}\psi_1^3 v dx=0 \big\}.
$$
From the simplicity of $\mu_1$ we have $H=\operatorname{span}\{\psi_1\}\oplus V$.
We introduce the quantity
$$
\mu_V=\inf \big\{ \|u\|^4:u\in V, \|u\|^4_{L^4}=1\big\}.
$$
Then
\begin{equation}\label{23}
\|u\|^4 \geq \mu_{V}\|u\|^4_{L^4},\quad \forall u\in V,
\end{equation}
and we have the following result.

\begin{lemma} \label{lem2}  
$\mu_1<\mu_V$.
\end{lemma}

\begin{proof} It is evident from \eqref{principal character} that 
$\mu_1\leq \mu_V$. Assume, by contradiction, that $\mu_1=\mu_V$. 
Then there exists a sequence $\{u_n\}\subseteq V$ such that 
$\|u_n\|_{L^4}=1$ for all $n\geq 1$, and $\|u_n\|^4\to  \mu_V=\mu_1$.
Since the sequence $\{u_n\}$ is bounded in $H$, we may assume that
\begin{equation}\label{18}
u_n \rightharpoonup u \quad \text{weakly in } H, \quad
u_n \to  u \quad \text{strongly in } L^4(\Omega).
\end{equation}
Thus, one has
\begin{gather*}
\|u\|_{L^4}=\lim_{n\to  +\infty} \|u_n\|_{L^4}=1 , \\
\mu_1\leq\|u\|^4\leq \liminf_{n\to  \infty} \|u_n\|^4
=\lim_{n\to  \infty}\|u_n\|^4=\mu_1.
\end{gather*}
So, $ \|u\|_{L^4}=1$ and $\|u\|^4=\mu_1$. This implies $u=\pm \psi_1$.

On the other hand,  from  $\{u_n\}\subseteq V$ it follows that
$\int_{\Omega} \psi_1^3 u_n =0$ for all $n\geq 1$. Combining this
 with \eqref{18} and H\"older's inequality, we have
\begin{align*}
\big|\int_{\Omega}\psi_1^3 u dx\big|
&= \big|\int_{\Omega}\psi_1^3 u dx-\int_{\Omega}\psi_1^3 u_n dx\big|
=\big|\int_{\Omega}\psi_1^3 (u- u_n) dx\big|\\
&\leq \int_{\Omega}\left|\psi_1^3 (u-u_n)\right| dx \\
&\leq \|\psi_1\|^3_{L^4}\|u_n-u\|_{L^4}\to  0,\quad \text{as } n\to  \infty.
\end{align*}
This is in direct contradiction to the fact $u=\pm \psi_1$. 
Hence $\mu_1<\mu_V$.
\end{proof}

\begin{proof}[Proof of Theorem \ref{thm1}]
 We shall divide the proof into four steps.
\smallskip

\noindent\textbf{Step 1.} The functional $I_{\mu}$ is bounded below in $H$ 
and $V$ and even coercive in $H$ and $V$. 
More specifically, there is a constant $\alpha$, independent of 
$\mu$, such that $\inf_{V} I_{\mu} \geq \alpha$.
From \eqref{9}, we obtain
\begin{equation}\label{24}
|F(x,t)|\leq \frac{ b\varepsilon}{4} |t|^4 +M_{\varepsilon}|t|,\quad
 \forall (x,t)\in \Omega\times {\mathbb{R}}.
\end{equation}
It follows from \eqref{sobolev insert}, \eqref{24} and H\"older inequality that
\begin{align*}
I_{\mu}(u)
&\geq  \frac{a}{2}\|u\|^2+\frac{b}{4}\|u\|^4
 -\frac{b(\mu+\varepsilon)}{4}\int_{\Omega}u^4dx
 -(M_{\varepsilon}|\Omega|^{1/2}+\|h\|_{L^2})\|u\|_{L^2} \\
&\geq  \frac{b}{4}(1-\frac{\mu+\varepsilon}{\mu_1})\|u\|^4
 -\tau_2(M_{\varepsilon}|\Omega|^{1/2}+\|h\|_{L^2})\|u\|,\quad \forall u\in H\,.
\end{align*}
Note that $\mu<\mu_1$. 
Then, for $0<\varepsilon <\mu_1-\mu$, $I_{\mu}$ is bounded below and even 
coercive in $H$. Similarly, for $0<\varepsilon<\mu_V -\mu_1$, 
\eqref{sobolev insert}, \eqref{23}, \eqref{24} and H\"older inequality lead to
\begin{align*}
I_{\mu_1}(v) 
&\geq \frac{a}{2}\|v\|^2+\frac{b}{4}\|v\|^4
 -\frac{b(\mu_1+\varepsilon)}{4}\int_{\Omega}v^4dx
 -(M_{\varepsilon}|\Omega|^{1/2}+\|h\|_{L^2})\|v\|_{L^2} \\
&\geq \frac{b}{4}(1-\frac{\mu_1+\varepsilon}{\mu_V})\|v\|^4
 -\tau_2(M_{\varepsilon}|\Omega|^{1/2}+\|h\|_{L^2})\|v\|, \quad \forall v\in V,
\end{align*}
which implies that $I_{\mu_1}$ is bounded below and coercive in $V$.
 Noting that $I_{\mu}\geq I_{\mu_1}$ for all $\mu<\mu_1,$ we deduce $I_{\mu}$ 
is coercive in $V$ and
\[
\inf_{V}I_{\mu}\geq \alpha:= \inf_{V}I_{\mu_1}.
\]
\smallskip

\noindent\textbf{Step 2.}
 If $\mu<\mu_1$ is sufficiently close to $\mu_1$, there exist two 
constants $t^-, t^+$ with $t^-<0<t^+$ such that 
$I_{\mu}(t^{\pm}\psi_1)<\alpha$.
Noting $\|\psi_1\|_{L^4}=1,\|\psi_1\|^4= \mu_1$
and then combining this with (H1), for $t\in \mathbb{R}$, we have
\begin{align*}
I_{\mu}(t\psi_1)
&= \frac{at^2}{2}\|\psi_1\|^2+\frac{bt^4}{4}\|\psi_1\|^4
 -\frac{b \mu t^4}{4}\int_{\Omega}\psi_1^4dx-\int_{\Omega}F(x,t\psi_1)dx \\
&= \frac{b(\mu_1-\mu)}{4}t^4-\Big(\int_{\Omega}F(x,t\psi_1)dx
 -\frac{a}{2}\sqrt{\mu_1}t^2 \Big).
\end{align*}
From (F2), taking a constant $t^+$ with $t^+>0$ large enough, we obtain
\begin{equation*}
\int_{\Omega}F(x,t^+\psi_1)dx-\frac{a}{2}\sqrt{\mu_1}(t^+)^2>-\alpha+1.
\end{equation*}
The above inequality reduces to
\begin{equation*}
I_{\mu}(t^+\psi_1) \leq \frac{b (\mu_1-\mu)}{4}(t^+)^4+\alpha-1.
\end{equation*}
Consequently, for $-\frac{4\mu_1}{{b(t^+)}^4}<\mu <\mu_1$, we obtain 
$I_{\mu}(t^+\psi_1) < \alpha$. 
The same conclusion holds for a constant $t^-$ with $t^-<0$.
\smallskip

\noindent\textbf{Step 3.}
Two solutions are obtained based on the coerciveness of $I_{\mu}$ and 
Ekeland's variational principle.
Set
\[
\Theta^{\pm}=\{u \in H: u=\pm t \psi_1 +v  \text{ with }\ t >0, v\in V\}.
\]
When $\mu <\mu_1$ is sufficiently close to $\mu_1$, from step 1 and step 2, 
$I_{\mu}$ is bounded below in $\Theta^{+}$ with
\[
-\infty < c^+:=\inf_{\Theta^{+}} I_{\mu}<\alpha.
\]
In $\Theta^{+}$, if we apply Ekeland's variational principle to $I_\mu$, 
there exists a sequence $\{u_n\}\subset \Theta^{+}$ such that 
$I_{\mu}(u_n)\to  c^+$ and $I'_{\mu}(u_n)\to  0$ as $n\to  \infty$.
By the coerciveness of $I_{\mu}$ in $H$, we deduce that $\{u_n\}$ is bounded.  
So, $\{u_n\}$ is a sequence satisfying \eqref{bound ps} so that
 Lemma \ref{lem1} implies $\{u_n\}$ has a convergent subsequence, say $\{u_n\}$ itself. 
Noting that $V=\partial \Theta^{+}$ and $\inf_{V}I_{\mu}\geq \alpha$ (step 1), 
we conclude that $\{u_n\}$ converges to an interior point $u^+ \in \Theta^{+}$,
that is, the infimum is attained in $\Theta^{+}$. 
Therefore, $I_{\mu}$ has a critical point $u^+$ as a local minimum in 
$\Theta^{+}$. Similarly, we obtain a critical point $u^-$ of $I_{\mu}$ as 
a local minimum in $\Theta^{-}$. Note that $\Theta^{+}\cap \Theta^{-}=\emptyset$
 which implies $u^+\neq u^-$, that is, $I_{\mu}$ has two different local 
minimum points.
\smallskip

\noindent\textbf{Step 4.}
 It follows from Theorem \ref{thm2} that $I_\mu$ has a third solution.
By Lemma \ref{lem1}, we see $I_\mu$ satisfies $(PS)$ condition.
 It follows from step 3 that $u^+, u^-$ are two different local minimum 
points. Consequently, Theorem \ref{thm2} shows that $I_{\mu}$ has a third critical point. 
\end{proof}

\subsection*{Acknowledgments}
This work is supported by National Natural Science Foundation of China
(No. 11471267), and by Science and Technology Researching Program of
Chongqing Educational Committee of China (Grant No.KJ130703).


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\end{document}
