\documentclass[reqno]{amsart}
\usepackage{hyperref}

\AtBeginDocument{{\noindent\small
\emph{Electronic Journal of Differential Equations},
Vol. 2009(2009), No. 93, pp. 1--12.\newline
ISSN: 1072-6691. URL: http://ejde.math.txstate.edu or http://ejde.math.unt.edu
\newline ftp ejde.math.txstate.edu}
\thanks{\copyright 2009 Texas State University - San Marcos.}
\vspace{8mm}}

\begin{document}
\title[\hfilneg EJDE-2009/93\hfil A biharmonic elliptic problem]
{A biharmonic elliptic problem with dependence on the gradient
 and the Laplacian}

\author[P. C. Carri\~ao, L. F. O. Faria, O. H. Miyagaki\hfil EJDE-2009/93\hfilneg]
{Paulo C. Carri\~ao, Luiz F. O. Faria, Ol\'impio H. Miyagaki}  % in alphabetical order

\address{Paulo C. Carri\~ao \newline
 Departamento de Matem\'atica, Universidade Federal de Minas Gerais\\
 31270-010 Belo Horizonte (MG), Brazil}
\email{carrion@mat.ufmg.br}

\address{Luiz F. O. Faria\newline
 Departamento de Matem\'atica, Universidade Federal de Juiz de Fora\\
 36036-330 Juiz de Fora (MG), Brazil}
\email{luiz.faria@ufjf.edu.br}

\address{Ol\'impio H. Miyagaki \newline
Departamento de Matem\'atica, Universidade Federal de Vi\c cosa \\
36571-000 Vi\c cosa (MG), Brazil}
\email{olimpio@ufv.br}

\thanks{Submitted March 22, 2009. Published August 6, 2009.}
\subjclass[2000]{31B30, 35G30, 35J40, 47H15}
\keywords{Biharmonic; Navier boundary condition; truncation techniques;
\hfill\break\indent iteration method}

\begin{abstract}
  We study the existence of solutions for nonlinear biharmonic
  equations that depend on the gradient and the Laplacian, under
  Navier boundary condition.
  Our main tools are an iterative scheme of the mountain pass
 ``aproximated'' solutions, and the truncation method developed
  by de Figueiredo, Girardi and Matzeu.
\end{abstract}

\maketitle
\numberwithin{equation}{section}
\newtheorem{theorem}{Theorem}[section]
\newtheorem{lemma}[theorem]{Lemma}
\newtheorem{remark}[theorem]{Remark}

\section{Introduction}

We prove the existence of nontrivial
solutions for the equation
\begin{equation}\label{nb}
\begin{gathered}
\Delta^{2}u+q\Delta u+\alpha(x)u=f(x,u,\nabla u,\Delta u)\quad
\text{in } \Omega\\
 u(x)=0, \quad \Delta u(x)=0\quad \text{on }  \partial \Omega,
 \end{gathered}
\end{equation}
where $\Delta^2$ is the biharmonic operator and
$\Omega\subset\mathbb{R}^{N}$, $N\geq 1$, is a bounded domain
with smooth boundary $\partial \Omega$.

The above  fourth-order semilinear elliptic problem, when $f$ does
not depend on derivatives of $u$, has been studied by many
authors; see  \cite{Arioli, Bernis, Noussair,  pevorst}
and references therein. In this case  variational
techniques are widely applied to obtain existence of solutions.

When  $\Omega=\mathbb{R}$ and $q >0$ the problem \eqref{nb} is is called
the Swift-Hohenberg equation, and for  $q>0$ it is called the
extended Fisher-Kolmogorov equation. For
this class of problems the existence of homoclinic, heteroclinic and
periodic solutions have been  obtained by several researchers mainly
when $f$ does not depend on derivatives; see e. g.
\cite{Terracini, Chap, GST, vivi,   Berg, Tersian}.
The reader is refereed to \cite{Aftabizadeh,
 Cosner-Fabry, Del pino-Manasevich, Lazer-Mckena2, Ma-Wang}
for the case $\Omega = (0,1)$ and $f$ depending on  the second order
derivative but not on the first derivative  of $u$.
Recently, the authors in \cite{Luiz} studied a situation where $f$
depends on the first and second order derivatives.
For studies with nonlinearities of the form $f(x,u,\Delta u)$
the reader is referred to
\cite{ed-fort-serrin, Micheletti-Pistoia, qian-li, Tarantello}
and references there in.

In our case, due to the presence of the gradient and
the Laplacian of $u$ in $f$, the problem is not variational whihc
creates additional difficulties. For instance the critical point
theory can not be applied directly. We recall that,  to overcome
this difficult, Xavier \cite{Xavier} and Yan
\cite{Yan} handled some semilinear elliptic problems of the
second order involving  the gradient by using monotone iterative methods.
We apply a technique developed by  De Figueiredo, Girard and
Matzeu \cite{FGM} (see also  Girard and  Matzeu \cite{gir})
which ``freezes'' the gradient variable and use truncation on the
nonlinearity $f$. Thus the new problem becomes  variational.
The idea of this approach is to consider a class of
problems through an iterative scheme where the approximated
problem has a nontrivial solution via mountain pass Theorem. Then
one obtains estimates  in $H^2(\Omega) \cap H^{1}_{0}(\Omega)
$-norm and $C^2$-norm. Passing to the limit in a sequence of the
approximated solutions we gets a solution of the original
problem. In general, a semilinear Navier fourth-order problem
is equivalent to the semilinear Dirichlet problem for a system
of two coupled  second order equations but it is not clear that
the truncation method works for the system.

To state our results, let us assume the following
conditions:


\begin{itemize}
\item[(A1)] $\alpha$ is a H\"older-continuous function.

\item[(A2)] There are positive constants a, b verifying
$0<a\leq\alpha(x)<b$,  $\forall x \in \mathbb{R}$.

\item[(A3)] $q\in(-\infty,2\sqrt{a})$.

\item[(F0)] $f:\Omega\times
\mathbb{R}\times\mathbb{R}^{N}\times\mathbb{R}\to \mathbb{R}$  is locally
Lipschitz continuous.

\item[(F1)] $
\lim_{t\to 0} f(x,t,\xi_{1},\xi_{2})/t=0$ uniformly
with respect to $x\in\Omega$, $\xi_{1}\in \mathbb{R}^{N}$  and
$\xi_{2}\in \mathbb{R}$.

\item[(F2)]
There exist $a_{1}>0$, $p\in (1,\frac{N+4}{N-4})$, ($N\geq 5$),
 $r_{1}$ and $r_{2}$ , such that $r:= r_{1} + r_{2}<1$ and
\[
|f(x,t,\xi_{1},\xi_{2})|\leq a_{1}(1+|t|^{p})(1+|\xi_{1}|^{r_{1}})
(1+|\xi_{2}|^{r_{2}}),
\]
for all $(x,t,\xi_{1},\xi_{2})\in \Omega\times\mathbb{R}^{N+2}$.

\item[(F3)] There exist $\theta>2$ and $t_{0}>0$ such that
\[
0<\theta F(x,t,\xi_{1},\xi_{2})\leq tf(x,t,\xi_{1},\xi_{2}),\quad
 \forall x \in \Omega, |t|\geq t_{0}, (\xi_{1},\xi_{2})
\in \mathbb{R}^{N+1},
\]
where
$F(x,t,\xi_{1},\xi_{2})=\int_{0}^{t}f(x,s,\xi_{1},\xi_{2})ds$.

\item[(F4)]
There exists  $a_{2},a_{3}>0$ such that
\[
F(x,t,\xi_{1},\xi_{2})\geq a_{2}|t|^{\theta}-a_{3}, \quad
\forall x\in \Omega,
(t,\xi_{1},\xi_{2})\in \mathbb{R}^{N+2}.\]
\end{itemize}

Denote by $y^{i,j}$, $(i=1,2,3$) the  vectors
 $$
y^{1,j}=(y^{j}_1,y_2,y_3),\quad
y^{2,j}=(y_1,y^{j}_2,y_3),\quad
y^{3,j}=(y_1,y_2, y^{j}_3) .
$$
For  $i,k=1,2,3$ and $j=1,2$, we define the  numbers:
$$
L_{\rho_{i}}=\sup\big\{
\frac{|f(x,y^{i,1})-f(x,y^{i,2})|}{|y^{1}_{i}-y^{2}_{i}|}:
(x,y^{i,j}) \in A_i \big\},
$$
where
$$
A_i=\{(x,y^{i,j})\in \Omega\times\mathbb{R}^{N+2}, \;
|y^{j}_i|\leq\rho_{i},\; |y_k|\leq\rho_{k} (i \neq k )\},
$$
for some constants $\rho_i> 0$.

\begin{itemize}
\item[(F5)] There exist positive numbers  $\rho_{i}$
($i=1,2,3$) depending on $q,\theta,a_{1},a_{2}$ and $a_{3}$, in an
explicit way, such that the above positive numbers  $L_{\rho_{i}}$
$(i=1,2,3)$ satisfy the relation
\[
(\tau_{1}L_{\rho_{1}}+\tau_{2}L_{\rho_{2}}+\tau_{3}
L_{\rho_{3}})\tau_{1}< \gamma,
\]
where  $\gamma$ is as in Lemma \ref{le0} and $\tau_{i}$
$(i=1,2,3)$ are the optimal constants  (that is, the smaller
constants) of the inequalities
\[
\Big(\int_{\Omega}|u|^{2}dx\Big)^{1/2}
\leq\tau_{1}\|u\|,\quad
\Big(\int_{\Omega}|\nabla u|^{2}dx\Big)^{1/2}\leq\tau_{2}\|u\|,\quad
\Big(\int_{\Omega}|\Delta u|^{2}dx\Big)^{1/2}\leq\tau_{3}\|u\|,
\]
where
$\|u\|^{2}=(u,u)$ and
$(u,v)=\int_{\Omega}(\Delta u\Delta v+\nabla u\nabla v+uv)dx$.
\end{itemize}

Under such hypotheses, we prove the following result.

\begin{theorem}\label{teo1}
If {\rm (A1)--(A3), (F0)--(F5)} hold,  then
there exists at least one classical solution of \eqref{nb}.
\end{theorem}


\noindent \textbf{Example:}
 Suppose $\beta$ and $\delta$
positive and continuous functions. If $f(x,t,\xi_1,\xi_2 )= \beta
(x)|t|t(1+|\xi_1|)^{1/4}(1+|\xi_2|)^{1/4}+\delta(x)t^3$, then it
satisfies all the conditions  (F0)--(F5).

\begin{remark} \label{rmk1}  \rm
If  $\Omega= \delta \Omega'$, with $\delta > 0$ and $\Omega'$ is
a bounded domain containing the origin, all functions verifying
the growth conditions (F1)--(F4) satisfy the condition (F5)
for $\delta$ small sufficient. It occurs because the constants
$\tau_i$ ($i=2,3$)  and  $L_{\rho_i}$ ($i=1,2,3$) do not increase
as $\delta$ approaches zero, and, by Poincar\'{e} inequality,
we can choose
$\tau_1 = (\frac{\delta (\mbox{diameter of }\Omega')}{w_N})^{1/N}$
with  ${w_N}$  the measure of the unity ball in $\mathbb{R}^N$.
\end{remark}

\section{Notation and a technical result}

Let $X\equiv H^2(\Omega) \cap H^{1}_{0}(\Omega)$,
which is a Hilbert space with inner product and norm given
in the previous section. Since  (\ref{nb}), in general, is not variational we use
a ``freezing'' technique whose formulation appears initially in
\cite{FGM}. This technique consists of associating to the
problem \eqref{nb} a family of problems without dependence
of $f$ in the gradient and  Laplacian of the solution. That is,
for each $w\in X $ fixed we consider the  ``freezed''  problem
given by
\begin{equation}
\begin{gathered}
\Delta^{2}u_{w}+q\Delta u_{w}+\alpha(x)u_{w}=f(x,u_{w},\nabla
w,\Delta w)\quad\text{in }  \Omega \\
 u_{w}(x)=0, \quad  \Delta u_{w}(x)=0 \quad \text{on } \partial
 \Omega.
\end{gathered}
\end{equation}


The nonexistence  of  a priori estimates, with respect to the
norms of the gradient and Laplacian of the solution,  is the main
difficulty for using variational techniques. Thus, we
consider, for each $R>0$ fixed, the truncated ``functions''
\[
f_{R}(x,t,\xi_{1},\xi_{2})
=f(x,t,\xi_{1}\varphi_{R}(\xi_{1}),\xi_{2}\varphi_{R}(\xi_{2})),
\]
 and
\[
F_{R}(x,t,\xi_{1},\xi_{2}) = \int_{0}^{t}f_{R}(x,s,\xi_{1},\xi_{2} )ds,
\]
where $\varphi_{R}
\in C^1(\mathbb{R})$, $| \varphi_{R} | \leq 1 $ and
$$
\varphi_{R}(\xi) = \begin{cases}
1 &\text{if }  |\xi|\leq R, \\
0 & \text{if }  | \xi|\geq R+1. \end{cases}
$$
This argument appears initially in \cite{Jin}.  See
also \cite{gir}.

\begin{remark}  \label{obs-trunc}\rm
Note that $|\xi\varphi_{R}(\xi)|\leq R+1$,
for all $\xi\in\mathbb{R}$.
\end{remark}

Thus, for each $w\in X$ and $R>0$ fixed, we consider ``truncated''
  and ``freezed'' problem, given by
\begin{equation}\label{biarmonic-rt}
\begin{gathered}
\Delta^{2}u^{R}_{w}+q\Delta
u^{R}_{w}+\alpha(x)u^{R}_{w}=f_{R}(x,u^{R}_{w},\nabla w,\Delta
w)\quad\text{in }  \Omega \\
 u^{R}_{w}(x)=0, \quad  \Delta u^{R}_{w}(x)=0 \quad \text{on }  \partial
 \Omega.
 \end{gathered}
\end{equation}
The  associated functional  $I_{w}^{R}:X\to \mathbb{R}$ is
\begin{equation}\label{func}
 I_{w}^{R}(v)=\frac{1}{2}\int_{\Omega}[(\Delta v)^{2}
-q(\nabla v)^{2}+\alpha(x)v^{2} ]dx
 - \int_{\Omega}F_{R}(x,v,\nabla w,\Delta w)dx.
\end{equation}
The following technical Lemma gives us a new and equivalent norm in
$X$.

\begin{lemma}\label{le0}
Suppose $\alpha$ and $q$ satisfy {\rm (A1)--(A3)}. Then there exist
positive constants $\eta$ and $\gamma$ such that
\[
\gamma\|u\|^{2}\leq \int_{\Omega}(\Delta u^{2}-q\nabla
u^{2}+\alpha(x)u^{2} )dx\leq\eta\|u\|^{2}, \quad
 \forall u \in H^{2}(\Omega).
\]
\end{lemma}

\begin{proof}
The constant $\eta$ is obtained taking $\eta = \max\{-q, b, 1 \} $.
To obtain $\gamma$,  notice that if $q <0$, it is sufficient to take
$\gamma = \min\{-q, a, 1 \}$.
In the case where $q\geq 0 $, and
$\Omega\subset \mathbb{R}$, $\gamma $  will be taken as in
\cite[Lemma 8]{Tersian}. For $\Omega\subset \mathbb{R}^{N},N>1 $,
 the proof can be adapted from  \cite[Lemma 8]{Tersian}.
\end{proof}

\section{Proof of main theorem}

We assume $N\geq 5$; the case $N \in [1,4]$ is easier.
The proof of  Theorem \ref{teo1} is achieved with several lemmas.
The following result establishes the mountain pass geometry for
the functional $I_{w}^{R}$.

\begin{lemma}\label{le1}
Let $w\in X $ and $R>0$ be fixed. Then
\begin{itemize}
 \item[(i)]
there exist positive constants $\rho=\rho_{R}$ and
$\alpha=\alpha_{R}$ such that $I_{w}^{R}(v)\geq\alpha$,
for all $v\in X$ with $ \|v\|=\rho$.

\item[ii)] fix  $v_{0}$ with $\|v_{0}\|=1 $; there is a $T>0$
 such that $I^{R}_{w}(tv_{0}) \leq 0$,  for all $t>T$.
\end{itemize}
\end{lemma}

\begin{proof}  By (F1), given any $\varepsilon>0 $ there exists  some
$\delta>0 $ such that $|v|<\delta$, implies
\begin{equation}
\label{eq1}
F_{R}(x,v,\nabla w,\Delta w)\leq \varepsilon\frac{v^{2}} {2}.
\end{equation}
Now, if $|v|\geq\delta $, by (F2) and by Remark
\ref{obs-trunc}, there exists
some constant $k=k(\delta)$ such that
\begin{equation}\label{eq2}
F_{R}(x,v,\nabla w,\Delta w)\leq k |v|^{p+1}(R+2)^{r}.
\end{equation}
Thus, by inequalities (\ref{eq1}) and \eqref{eq2} and by Lemma
\ref{le0} we have
\[
I_{w}^{R}(v)
\geq \frac{\gamma}{2} \|v\|^{2}-\frac{\varepsilon}{2}
 \int_{\Omega}|v|^{2}dx-k(R+2)^{r}\int_{\Omega}|v|^{p+1}dx.
\]
So, by the Sobolev embedding Theorem we have
\[
I_{w}^{R}(v) \geq  \frac{1}{2} (\gamma
-C\varepsilon) \|v\|^{2}-kC(R+2)^{r}\|v\|^{p+1},
\]
 for some positive constant $C$. Then for a $\varepsilon$
small sufficient, we can choose $\rho=\rho_{R}$ and
$\alpha=\alpha_{R}$, both independent of $w$, such that the
first part of the result holds.

Now, take an arbitrary $v_{0}\in X$ with $\|v_{0}\|=1$. By
(F4) and Lemma \ref{le0}
\[
I_{w}^{R}(tv_{0}) \leq \frac{\eta |t|^{2}} {2}\|v_{0}\|^{2} -
a_{2}|t|^{\theta}\int_{\Omega}|v_{0}|^{\theta}dx+a_{3}|\Omega |.
\]
Since $\theta >2$, it is possible to choose $T>0$ such that
$I^{R}_{w}(tv_{0}) \leq 0$,  for all $t>T $.
\end{proof}

\begin{lemma}\label{le2}
For any $w\in X $, $R>0 $, problem \eqref{biarmonic-rt} has a
nontrivial weak solution.
\end{lemma}

\begin{proof} First of all, from Lemma \ref{le0}, (F0), (F1) and
(F2), the functional $I_{w}^{R}$ is in $C^1(X,\mathbb{R})$; see e.g.
\cite{ambrab}.

\subsection*{Claim} %\label{ob1}
$I_{w}^{R}$ satisfies the Palais-Smale condition;
that is, every sequence $(u_n)\subset X$ such that
$$
I_{w}^{R}(u_n)\to c\quad\text{and}\quad I_{w}^{'R}(u_n)\to 0,
\quad\text{as } n\to \infty,
$$
for some constant $c$, contains a convergent subsequence.

\subsection*{Verification of the Claim}
Note that
$$
I_{w}^{R}(u_n)-\frac{1}{\theta}\langle I_{w} ^ {' R}(u_n),u_n\rangle \leq
c+\|u_n \|, \quad \forall n>n_{0}.
$$
since $\theta>2 $, from  Lemma \ref{le0}, it is standard to prove that,
$$
\|u_{n}\|<C, \quad C>0.
$$
By the Rellich-Kondrachov  Theorem, up to a subsequence, there exists
$u\in X$ such that
\[
u_{n}\to u \quad\text{in }L^{p+1}(\Omega)\quad\text{as }  n\to \infty.
 \]
So, as $ n\to \infty$, we have
$$
f_{R}(x,u_{n},\nabla
w,\Delta w)\to f_{R}(x,u,\nabla w,\Delta w) \quad
\text{in } L^{\frac{p+1}{p}} (\Omega).
$$
Therefore,
 \begin{equation} \label{2b}
\int_{\Omega} [f_R(x,u_n,\nabla w,\Delta w)-f_R(x,u,\nabla w,
 \Delta w)] (u_n -u)dx
\to 0, \quad \text{as } n\to \infty.
\end{equation}
Since $(I_{w} ^ {' R}(u_n) -I_{w} ^ {' R}(u)) \to - I_{w}^ {' R}(u)$
and $u_{n}\rightharpoonup u$
weakly in $X$, we have
\begin{equation} \label{2a}
\langle I_{w} ^ {' R}(u_n) -I_{w} ^ {' R}(u),
 u_n-u\rangle \to 0, \quad \text{as }  n\to \infty.
\end{equation}

Notice that by Lemma \ref{le0}
\begin{align*}
&\langle I_{w} ^ {' R}(u_n) -I_{w} ^ {' R}(u),
u_n-u\rangle+  \int_{\Omega}
[f_R(x,u_n,\nabla w,\Delta w)-f_R(x,u,\nabla w,\Delta w)] (u_n - u)dx \\
&\geq \gamma \|u_n -u\|^2.
\end{align*}
Using \eqref{2b} and \eqref{2a} in the above inequality, we obtain
that $u_n \to u $(strong) in  $X$ as $n\to \infty$. Thus, we
conclude that the statement is true.

Applying the mountain pass Theorem, due to
Ambrosetti-Rabinowitz \cite{ambrab},  there exists $u_w^R \neq 0 $
weak solution to problem
\eqref{biarmonic-rt}
\end{proof}

\begin{lemma}\label{le3}
Let $R>0$ be fixed. Then there exist positive constants
$d_{1}:=d_{1}(R) $, $d_{2}:=d_{2}(R) $, independent of $w$, such
that
\[
d_{2}\leq\|u_{w}^{R}\|\leq d_{1},
\]
for all solution $u^{R}_{w}$ obtained in  Lemma \ref{le2}.
\end{lemma}

\begin{proof} Notice that
$$
I_{w}^{R}(u_w^R) \leq \max_{t\geq 0}I_{w}^{R}(tv_0),
$$
with $v_{0}$ given as in Lemma  \ref{le1}.
 From (F4) and Lemma \ref{le0} we obtain
$$
I_{w}^{R}(tv_0)\leq \frac{t^2}{2}\eta -a_{2}|t|^{\theta}
\int_{\Omega}|v_{0}|^{\theta}dx+a_{3}|\Omega |.
$$
Since $\theta>2$ and  $|v_{0}|_{\theta}\neq 0 $, the map
$$
t\in\mathbb{R}\mapsto \eta\frac{t^{2}} {2}-a_{2}|t|
^{\theta}\int_{\Omega}|v_{0}|^{\theta}dx+a_{3}|\Omega|
$$
attains a positive maximum, independent of $w$ and $R$. So we
get a constant $C$ such that
\begin{equation}\label{fuc}
I^{R}_{w}(u_{w}^{R}) \leq C.
\end{equation}
Now, define
$$
|||u|||^{2} = \int_{\Omega}(\Delta u^{2}-q\nabla u^{2}
+\alpha(x)u^{2} )dx,
$$
which  by Lemma \ref{le0} is an equivalent norm in $X$.
By  (\ref{fuc}), we have
\begin{equation} \label{3.55}
\frac{1}{2}|||u_{w}^R|||^{2}\leq C
+\int_{\Omega}F_{R}(x,u_{w}^R,\nabla w,\Delta w),\quad C>0.
\end{equation}

Let $t_{0}$ be as in condition (F3), and define
$D:=\{x\in\Omega;|u_{w}^R(x)|>t_{0} \}$. Keeping in mind that
$u_w^R$ is a solution from (F2) and (F3) and by Remark
\ref{obs-trunc}, we have
\begin{align*}
\int_{\Omega}F_{R}(x,u_{w}^R,\nabla w,\Delta
w)&=\int_{\Omega\backslash
D}F_{R}(x,u_{w}^R,\nabla w,\Delta w)+\int_{D}F_{R}(x,u_{w}^R,\nabla w,\Delta w) \\
& \leq a_{1}(R+2)^{r}\Big(t_{0}+\frac{|t_{0}|^{p+1}}
{p+1}\Big)|\Omega\backslash
D|+\frac{1}{\theta}|||u_{w}^R|||^{2}.
\end{align*}
Returning to equation (\ref{3.55}) we have
\[
\frac{1}{2} || | u_{w}^R|||^{2}\leq C+
a_{1}(R+2)^{r}\Big(t_{0}+\frac{|t_{0}|^{p+1}}
{p+1}\Big)|\Omega\backslash
D|+\frac{1}{\theta}|||u_{w}^R|||^{2},
\]
where $|\Omega \backslash D|$ denotes the Lebesgue measure in
$\mathbb{R}^N$ of the set $\Omega \backslash D$.
Again by Lemma \ref{le0}, we have
\[
\gamma\big(\frac{1}{2}-\frac{1}{\theta}\big) \| u_{w}^R\|^{2}
\leq\big(\frac{1}{2}-\frac{1}{\theta}\big) ||| u_{w}^R|||^{2}
\leq C+ a_{1}(R+2)^{r}\big(t_{0}+\frac{|t_{0}|^{p+1}}
{p+1}\big)|\Omega\backslash D |.
\]
Thus, we can conclude that exists $c_1> 0$ such that
$$
\gamma\big(\frac{1}{2}-\frac{1}{\theta}\big)\|u_w^R\|^2 <c_1(R+2)^{r};
$$
that is,
$\|u_w^R\|\leq d_1$, for some $d_1=d_1(R)>0$.

Now, we shall prove that there exists $d_2>0$ such that
$\|u_w^R\|>d_2$. In fact, notice that
\begin{equation} \label{2c}
 I_{w} ^ {'R}(u_w^R)(u_w^R)=0,
\end{equation}
and from (F1) and (F2), given $\varepsilon>0$, there exists
$C_\varepsilon>0$ such that
\begin{equation} \label{d}
|f_R(x,u_w^R,\nabla w,\Delta w)|\leq \varepsilon
|u_w^R|+C_{\varepsilon}|u_w^R|^{p}(R+2)^{r}.
\end{equation}
Inserting $(\ref{d})$ in $(\ref{2c})$ and using Lemma
\ref{le0}, we have
$$
\gamma\|u_{w}^R\|^{2}\leq C_{1}\varepsilon
\|u_{w}^R\|^2+C_{2}C_{\varepsilon}\|u_{w}^R\|^{p+1}(R+2)^{R},
$$
for some constants $C_1, C_2 \geq 0$.
Therefore, there exists $d_{2}>0$ such that
$\|u_{w}^{R}\|\geq d_{2}$. This completes the proof.
\end{proof}

\begin{lemma}\label{le4}
Choose $w\in C^{4,\alpha}(\overline{\Omega}) $, for some
$\alpha\in(0,1)$, and let $R>0$ be fixed. If $u_{w}^{R}\in X$
 is a weak solution of problem \eqref{biarmonic-rt}, then
$u_{w}^{R}\in C^{4,\beta}(\overline{\Omega}) $, for some $\beta
\in(0,1) $, and $\Delta(u_{w}^{R})(x)=0$ if $x\in \partial\Omega$.
\end{lemma}

 \begin{proof}  Let $u_w^R\in X$ be a weak solution of
\eqref{biarmonic-rt}. Define
$v=\Delta u_w^R $ and
$$
g(x)=f_R(x,u_w^R,\nabla w, \Delta w)-q\Delta u_w^R-\alpha(x)u_w^R.
$$
By hypotheses (F2), and the Sobolev embedding, notice that
$g(x)\in L^2(\Omega)$. So, $v$ is a weak solution of
$$
\Delta v=g(x),\quad\text{in } \Omega,
$$
in the following sense: For
$\phi\in C^\infty_c(\Omega) $, we have
$$
\int_{\Omega}v\Delta \phi dx=\int_\Omega g\phi dx.
$$
 From Agmon \cite[Theorem 7.1']{Ag}, we have that
$v\in H^2_{\rm loc}(\Omega)$. Therefore,
$u_w^R\in H^4_{\rm loc}(\Omega)$.

Fix $\phi\in C^\infty_c(\Omega)$, since  $u_w^R\in X$  is a weak
solution of problem \eqref{biarmonic-rt}, we have
\begin{equation}\label{vb111}
\int_\Omega\Delta u_w^R\Delta\phi dx -q\int_\Omega\nabla
u_w^R\nabla\phi dx+\int_\Omega \alpha(x) u_w^R\phi dx=\int_\Omega
f_R(x,u_w^R,\nabla w, \Delta w)\phi dx.
\end{equation}
But $\mathop{\rm supp}\phi\subset\subset\Omega $, so
$$
\int_\Omega(\Delta^2 u_w^R + q\Delta u_w^R+ \alpha(x) u_w^R)\phi
dx=\int_\Omega f_R(x,u_w^R,\nabla w, \Delta w)\phi dx.
$$
From the denseness of $C^\infty_c(\Omega)$ in
$X=H^2(\Omega)\cap H^1_0(\Omega)$ we conclude that
\begin{equation}\label{vb11}
\int_\Omega(\Delta^2 u_w^R +q\Delta
u_w^R+ \alpha(x) u_w^R)\phi dx=\int_\Omega f_R(x,u_w^R,\nabla w,
\Delta w)\phi dx\quad  \forall\phi\in X.
\end{equation}
The Green identities guarantees
\begin{gather}\label{vb22}
\int_\Omega(\Delta u_w^R\Delta\phi - \phi\Delta^2u_w^R)
dx=\int_{\partial\Omega}\Big(\Delta
u_w^R\frac{\partial\phi}{\partial\nu}-\phi\frac{\partial(\Delta
u_w^R)} {\partial\nu}\Big) ds
=\int_{\partial\Omega}\Delta
u_w^R\frac{\partial\phi}{\partial\nu}ds,\\
\label{vb3}
q\int_\Omega\Delta u_w^R\phi
dx=q\int_{\partial\Omega}\phi\frac{\partial u_w^R}{\partial\nu}ds
-q\int_\Omega\nabla u_w^R\nabla\phi dx.
\end{gather}
So, combining  (\ref{vb111}), (\ref{vb11}), (\ref{vb22})
and (\ref{vb3}), we have
\begin{equation}\label{vb333}
\int_{\partial\Omega}\Delta
u_w^R\frac{\partial\phi}{\partial\nu}ds=0.
\end{equation}
 From (\ref{vb11}), we obtain that
\begin{equation}\label{vb4}
\Delta^2 u_w^R + q\Delta
u_w^R+ \alpha(x) u_w^R  = f_R(x,u_w^R,\nabla w, \Delta w)
\quad\text{a.e. in }\Omega.
\end{equation}
By  Green's identity,
$$
\int_\Omega\Delta^2 u_w^R\Delta u_w^Rdx=
-\int_\Omega (\nabla\Delta
u_w^R)^2dx+\int_{\partial\Omega}\frac{\partial \Delta u_w^R}
{\partial\nu}\Delta u_w^Rds.
$$
By (\ref{vb333}), we obtain
\begin{equation}\label{p}
\int_\Omega\Delta^2 u_w^R\Delta u_w^Rdx=-\int_\Omega (\nabla\Delta
u_w^R)^2dx.
\end{equation}
By Green's identity,
$$
\int_\Omega\Delta u_w^R u_w^Rdx=-\int_\Omega (\nabla u_w^R)^2dx+
\int_{\partial\Omega}\frac{\partial u_w^R}{\partial\nu} u_w^Rds\,.
$$
Since $u_w^R\in H_0^1(\Omega)$, we get
\begin{equation}\label{o}
\int_\Omega\Delta u_w^R u_w^Rdx=-\int_\Omega
(\nabla u_w^R)^2dx.
\end{equation}
Multiplying $\Delta u_w^R$  equation  (\ref{vb4}), and integrating
by parts and using  (\ref{p}) and (\ref{o}), we obtain
\begin{equation}\label{vb2}
\begin{aligned}
&-\int_\Omega (\nabla\Delta u_w^R)^2 dx +q\int_\Omega(\Delta
u_w^R)^2 dx-\int_\Omega \alpha(x)(\nabla u_w^R)^2 dx\\
&=\int_\Omega f_R(x,u_w^R,\nabla w, \Delta w)\Delta u_w^R dx
\end{aligned}
\end{equation}
By (F2) and Sobolev embbedding we can assume that
$$
\Big(\int_\Omega (f_R(x,u_w^R,\nabla w, \Delta w))^2 dx\Big)^{1/2}
<\infty\,.
$$
Thus, from (\ref{vb2})  we have
$\|u_w^R\|_{W^{3,2}(\Omega)}<\infty$.

Let be $\varphi\in C_c^1(\mathbb{R}^N)$. Integrating by parts, we have
$$
\int_\Omega\Delta u_w^R \frac{\partial
\varphi}{\partial x_i}dx=-\int_\Omega \varphi \frac{\partial
 \Delta u_w^R}{\partial x_i}+\int_{\partial\Omega}\Delta u_w^R
\varphi \nu^ids.
$$
Then,
$$
\big|\int_\Omega\Delta u_w^R \frac{\partial \varphi}{\partial x_i}dx\big|
\leq\big|\int_\Omega \varphi \frac{\partial
\Delta u_w^R}{\partial x_i}dx\big|
\leq \|u_w^R\|_{W^{3,2}(\Omega)}|\varphi|_{L^2(\Omega)}.
$$
Now, by \cite[ Prop IX.18]{BrezisAF} we obtain
\begin{equation}\label{equiv}
\Delta u_w^R\in H_0^1(\Omega).
\end{equation}
Now, let us consider the following notation
\begin{gather*}
v=\Delta u_w^R+qu_w^R, \\
g(x)=f_R(x,u_w^R,\nabla w, \Delta w)-\alpha(x)u_w^R.
\end{gather*}
Notice that $v$ and $u_w^R $ are solutions in the weak sense of
the respective differential equations with Dirichlet boundary
condition, namely,
\begin{equation} \label{nov1}
\begin{gathered}
\Delta v=g(x),\quad\text{in }  \Omega \\
 v(x)=0, \quad \text{on }  \partial\Omega,
\end{gathered}
\end{equation}
and
\begin{equation} \label{nov}
\begin{gathered}
\Delta u_{w}^R+qu_w^R=v(x),\quad\text{in }  \Omega \\
 u_{w}^R(x)=0, \quad \text{on }  \partial\Omega.
\end{gathered}
\end{equation}
By the Sobolev embedding, we have
$u_w^R\in L^{q}(\Omega)$, with $q=2N/(N-4)$. By
(F2), we have that $g\in
L^s(\Omega)$ with $s=\frac{q}{p}$, where $p$ is given in (F2).

We want to show that $u_w^R\in W^{4,r}(\Omega) $, for some $r$
such that $4r>N $. If $4s>N $, it is sufficient to take $r=s$. In
fact, applying  Agmon \cite[Theorem 8.2]{Ag}, we have
$u_w^R\in W^{4,r}(\Omega)$.
Now, suppose that $4s <N$. By the Sobolev embedding,
$$
u_w^R\in L^{q_1}(\Omega), \quad\text{where }q_1=\frac{Ns}{N-4s}.
$$
By  (F2), we have $g\in L^{s_1}$ with $s_1=q_1/p$.

 From  \cite[Theorem 8.2]{Ag}, we have  $v\in W^{2,s_1}(\Omega)$
and $u_w^R\in W^{4,s_1}(\Omega)$.
Since $1 <p <\frac{N+4}{N-4} $, there exists a  $\epsilon>0 $ such
that
\[
s=(1+\epsilon)\frac{2N}{N+4}.
\]
Thus,
\[
\frac{s_{1}} {s}=\frac{q_{1}} {q}=\frac{sN}{N-4s}\frac{N-4}{2N}
=(1+\epsilon)\frac{N(N-4)}{(N+4)(N-4s)}.
\]
But notice that (it is sufficient we substitute
$s=(1+\epsilon)2N/(N+4))$,
$$
\frac{N(N-4)} {(N+4)(N-4s)} >1.
$$
Therefore, $s_1/s>1+\epsilon$.
This argument is known as a  \emph{bootstrap}.

If $4s_1 <N $, applying  again the bootstrap  argument, we
obtain
$u_w^R\in W^{4,s_2}$, where
$$
s_2=\frac{Ns_1}{p(N-4s_1)}.
$$
Therefore,
$$
\frac{s_2}{s_1}=\frac{Ns_1(N-4s)} {Ns(N-4s_1)}>
(1+\epsilon)\frac{N-4s}{N-4s_1}>(1+\epsilon).
$$
We can repeat this last argument a finite times to obtain that
$u_w^R\in
W^{4,r}(\Omega) $, for some $r$ such that $4r\geq N $.

For the case $4r=N $, since $g\in L^{r}(\Omega) $, we have that
$g\in L^{k}(\Omega)$ for some $k <r$ such that $(1+\epsilon)k>r$.
Applying again the  bootstrap argument, we conclude
that $u_w^R\in W^{4,r}(\Omega)$, with $4r>N $.

Therefore, we can apply the Sobolev-Morrey Theorem to show that
$u_w^R\in C^{\alpha}(\overline{\Omega}) $, for some
$\alpha\in (0,1) $. By (F0) and $(A1) $, we have that
$$
g(x)=f_R(x,u_w^R,\nabla w, \Delta w)
-\alpha(x)u_w^R\in C^\beta(\overline{\Omega}), \quad
\text{for some } \beta\in (0,1).
$$
By applying the Schauder
estimates in (\ref{nov1}), we obtain that
$v \in C^{2,\beta}(\overline{\Omega})$.
By applying the Schauder estimates again, in (\ref{nov}), we
obtain
\begin{equation}\label{equiv2} u \in
C^{4,\beta}(\overline{\Omega}).
\end{equation}
To conclude, notice that by (\ref{equiv}) and
(\ref{equiv2}), we have
$\Delta u_w^R(x)=0$, if $x\in\partial\Omega$.
 \end{proof}

\begin{lemma}\label{le5}
There exist positive constants $\mu_{0} $, $\mu_{1}$ and
$\mu_{2}$, independent of $R>0 $ and  of $w\in X$, such that
\begin{gather*}
\|u_{w}^{R}\|_{C^{0}} \leq\mu_{0}(R+2)^{r}, \\
\|\nabla(u_{w}^{R}) \|_{C^{0}} \leq\mu_{1}(R+2)^{r}, \\
\|\Delta(u_{w}^{R}) \|_{C^{0}} \leq\mu_{2}(R+2)^{r}\,.
\end{gather*}
Also, there exists $\overline{R}>0$ such that
$\mu_{i}(\overline{R}+2)^{r}\leq \overline{R}$, for $i=0,1,2$.
\end{lemma}

\begin{proof} This result follows combining  Lemma \ref{le3}
and the results of the Sobolev embedding by arguing as in the
proof  Lemma \ref{le4}.

To obtain $\overline{R}>0 $ such that
$\mu_{i}(\overline{R}+2)^{r}\leq \overline{R}$, it is
sufficient to observe that $r <1 $, and therefore
$$
\frac{\mu_{i}} {\overline{R}^{1-r}}
\Big(\frac{\overline{R}+2}{\overline{R}} \Big)^{r}
\leq 1
$$
for $\overline{R}$ sufficiently large.
\end{proof}

Now, let us ``construct'' a nontrivial solution for  problem
 \eqref{nb}. Consider the following problem:
Let $u_0\in X\cap C^{4,\lambda}(\overline{\Omega})$,
$\lambda\in(0,1)$, and $u_{n}$ ($n=1,2,\ldots $) be a weak
solution of the problem $(P_{n}) $, that is, problem
\eqref{biarmonic-rt}, with $w=u_{n-1}$,
 which was found by the
mountain pass Theorem in Lemma \ref{le2} and $R=\overline{R}$
obtained in Lemma \ref{le5}.

Note that from Lemma \ref{le4} we have
$u_{n} \in C^{4}(\overline{\Omega})$ and from Lemmas \ref{le3} and
\ref{le5}, we infer that
$\|u_{n}\|\geq d_{2}$
and
\[
\|u_{n}\|_{C^{0}}, \| \nabla u_{n}\|_{C^{0}}, \| \Delta u_{n}\|_{C^{0}} \leq
\overline{R},
\]
respectively. Thus,
\begin{align*}
f_{\overline{R}} (x,u_n,\nabla u_{n-1},\Delta u_{n-1})
& = f(x,u_{n},\nabla u_{n-1}\varphi_{\overline{R}}(\nabla u_{n-1}), \Delta
u_{n-1}\varphi_{\overline{R}}(\Delta u_{n-1})) \\
& = f(x,u_{n},\nabla u_{n-1},\Delta u_{n-1}).
\end{align*}
So, $u_{n}$ is a weak solution of problem $(P_{n}) $.

\begin{remark} \label{rmk3} \rm
 When   the diameter of $\Omega$  approaches zero,
 by an easy calculation in the proof of Lemma \ref{le5},
it is possible to choose $\mu_{i}$ ($i=0, 1, 2$)
sufficiently small.
\end{remark}

\begin{lemma}\label{le7}
 In  hypothesis {\rm (F5)}, let us take
\begin{gather*}
\rho_{1}=\inf\{k_{1}: \|u_{n}\|_{C^{0}} \leq k_{1},\;\forall\;
n\in \mathbb{N} \} >0, \\
\rho_{2}=\inf\{k_{2}: \|\nabla u_{n}\|_{C^{0}} \leq k_{2},\;\forall\;
  n\in \mathbb{N} \} >0, \\
\rho_{3}=\inf\{k_{3}: \|\Delta u_{n}\|_{C^{0}} \leq k_{3},\;\forall\;
  n\in \mathbb{N} \}>0.
\end{gather*}
Then $\{u_{n} \} $ converges strongly in $X$.
\end{lemma}

\begin{remark} \label{rmk4}  \rm
We recall that the constant $d_1$ (Lemma\ \ref{le3}) is obtained
using only the conditions (F1)--(F4), and the constants
$\rho_1$, $\rho_2$, $\rho_3$ are exhibited combining the constant
$d_1$ with the Sobolev embedding constants. Thus, as is pointed
out in \cite{gir}, the  condition (F5) can be read as a constraint
on the growth coefficients of $f$ with respect to dimension $N$.
\end{remark}

 \begin{proof}[Proof of Lemma \ref{le7}]
In this proof we will use a  similar argument that used in
\cite{FGM} and \cite{gir}. Let $u_{n}$ and $u_{n+1}$ be a weak
solutions of problems $(P_{n})$ and $(P_{n+1})$,
respectively. Then, multiplying $(P_{n+1})$ resp.
$(P_{n})$ by $(u_{n+1}-u_{n})$ and integrating by parts,
and applying
 Lemma  \ref{le0} we obtain
\begin{align*}
&\gamma\|u_{n+1}-u_{n}\|^{2}\\
& \leq \int_{\Omega}[f(x,u_{n+1},\nabla u_{n},\Delta u_{n})
-f(x,u_{n},\nabla u_{n},\Delta u_n)](u_{n+1}-u_{n} )dx \\
&\quad +\int_{\Omega}[f(x,u_{n},\nabla u_{n},\Delta u_{n})
-f(x,u_{n},\nabla u_{n-1},\Delta u_{n})](u_{n+1}-u_{n} )dx \\
&\quad +\int_{\Omega}[f(x,u_{n},\nabla u_{n-1},\Delta u_{n})
-f(x,u_{n},\nabla u_{n-1},\Delta u_{n-1})](u_{n+1}-u_{n}
)dx.
\end{align*}
Thus, by  (F5) and  the H\"older inequality we
obtain
\begin{align*}
\gamma\|u_{n+1}-u_{n}\|^{2}
 & \leq  \tau_{1}^{2} L_{\rho_{1}} \|u_{n+1}-u_{n}\|^{2}+\tau_{1}\tau_{2}L_{\rho_{2}} \|
u_{n} - u_{n-1} \| \| u_{n+1} - u_{n}\| \\
&\quad +  \tau_{1}\tau_{3}L_{\rho_{3}} \|u_{n}-u_{n-1} \| \| u_{n+1} -
u_{n} \|.
\end{align*}
Therefore,
\begin{equation} \label{tt}
\|u_{n+1}-u_{n}\|\leq
\frac{(\tau_{1}\tau_{2}L_{\rho_{2} }+\tau_{1}\tau_{3}L_{\rho_{3}
})} {\gamma - \tau_{1}^{2}L_{\rho_{1}}} \|u_{n}-u_{n-1} \|.
\end{equation}
Hence it follows that the sequence ${u_{n}}$ converges strongly to
function $u$, in $X$.
\end{proof}

\subsection*{Proof of Theorem \ref{teo1}}
First of all, as before, we  obtain that $\|u_{n}\|\geq d_{2}>0 $.
Also, we see that,
\[
\|u_{n}\|_{C^{0}},\quad \|\nabla u_{n}\|_{C^{0}}, \quad
\|\Delta u_{n}\|_{C^{0}}
\]
are uniformly bounded.
Now, from $(P_{n}) $, notice that
$v_{n}=\Delta u_{n}$ verifies the equation
\[
\Delta v_{n}=h(x), \quad x \in \overline{\Omega},
\]
where
$$
h(x)=f(x,u_{n},\nabla u_{n-1},\Delta u_{n-1}) -q\Delta
u_{n}-\alpha(x)u_{n}.
$$
Since $\|h\|_{C^{\beta}} \leq C $, for
some positive constant $C$, by the Schauder Theorem  follows that
there exists a constant $C> 0$ such that
$\|v_{n}\|_{C^{2,\beta}} \leq C$;
therefore,
\[
\|u_{n}\|_{C^{4,\beta}} \leq C.
\]
From  Arzela-Ascoli Theorem, passing to a subsequence, if
necessary, we conclude that
$$
\frac{\partial^{j}} {\partial
x_{i}^{j} }u_{n}\to \frac{\partial^{j}} {\partial
x_{i}^{j} }u, \quad\text{as } n\to \infty,
$$
uniformly
in $\overline{\Omega}$ for $j=0,1,\ldots,4$ and $i=1,\ldots,N $.
Actually, from Lemma \ref{le7}, all the subsequences of
$\frac{\partial^{j}} {\partial x_{i}^{j} }u_{n} $ have the same
limit, so the whole sequence
$$
\frac{\partial^{j}} {\partial x_{i}^{j} }u_{n}\to
\frac{\partial^{j}} {\partial x_{i}^{j} }u,\quad \text{ as } n
\to \infty,\text{ for } j=0,1, \ldots, 4.
$$
Therefore, passing to the limit in $(P_{n})$, we obtain  that $u$
is a classical solution of \eqref{nb}. Hence, the proof
of Theorem \ref{teo1} is complete.

\subsection*{Acknowledgments}
L. Faria was supported in part by FAPEMIG - Brazil.
O.  Miyagaki was supported in part by CNPq - Brazil,
INCTmat-CNPQ- MCT/Brazil, Fapemig CEX APQ
0609-5.01/07 and
CAPES Pro Equipamentos 01/2007.


\begin{thebibliography}{99}

\bibitem{Aftabizadeh} A. R. Aftabizadeh;
 \emph{Existence and uniqueness
theorem for fourth-order boundary value problems}, J. Math. Anal.
Appl. 116 (1986), 416--426.

\bibitem{Ag} S. Agmon;
\emph{The $L\sb{p}$ approach to
the Dirichlet problem. I. Regularity theorems}, Ann. Scuola Norm.
Sup. Pisa (3) 13 (1959), 405--448.

\bibitem{ambrab} A. Ambrosetti and P. H. Rabinowitz;
\emph{Dual variational methods in critical point theory and
applications}, J. Funct. Anal. 14 (1973), 349--381.

\bibitem{Arioli} G. Arioli and  F. Gazzola, H. Ch. Grunau and E.
Mitidieri;
\emph{A semilinear fourth order elliptic problem with
exponential nonlinearity, } SIAM J. Math. Anal. 36 (2005),
1226--1258.

\bibitem{Bernis}  F. Bernis, J. Garcia Azorero and I. Peral;
\emph{Existence and multiplicity of nontrivial solutions in
semilinear critical problem of fourth order,} Adv. Diff. Eqns. 1
(1996), 219--240.

\bibitem{Terracini}D. Bonheure, L. Sanchez, M. Tarallo and
S. Terracini;
\emph{Heteroclinic
connections between nonconsecutive equilibria of a fourth order
differential equation}, Calc. Var. 17 (2003), 341--356.

\bibitem{BrezisAF} H. Brezis;
\emph{Analyse fonctionnelle th\'eorie et
applications}, Masson, Paris, (1983).

\bibitem{Luiz} P. C. Carri\~ao,  L. F. O. Faria and   O. H.
Miyagaki;
 \emph{Periodic solutions for extended Fisher-Kolmogorov
and Swift-Hohenberg equations by truncature techniques}, Nonlinear
Anal. 67 (2007), 3076--3083.

\bibitem{Chap}  J. Chaparova;
 \emph{Existence and numerical aproximations of periodic
solutions of semilinear fourth-order differential equations},  J.
Math. Anal. Appl. 273 (2002), 121--136.

\bibitem{Cosner-Fabry} C. De Coster, C. Fabry and  F. Munyamarere;
\emph{Nonresonance conditions for fourth-order nonlinear boundary value problems},
Internat. J. Math. Sci. 17 (1994), 725--740.

\bibitem{Del pino-Manasevich} M. A. Del Pino  and R. F Manasevich;
\emph{Existence for a fourth-order nonlinear boundary problem under
a two-parameter nonresonance contition}, Proc. Amer. Math. Soc.
112 (1991), 81--86.

\bibitem{FGM} D. De Figueiredo, M. Girardi and M. Matzeu;
\emph{Semilinear elliptic equations with dependence on the
gradient via mountain pass techniques}, Differential and Integral
Equations 17 (2004), 119--126.

\bibitem{ed-fort-serrin} D. E. Edmunds, D. Fortunato and
E. Jannelli;
\emph{Critical exponents, critical dimensions and the
biharmonic operator}, Arch. Rational Mech. Anal. 112 (1990), no.
3, 269--289.

\bibitem{gir}  M. Girardi and M. Matzeu;
\emph{Positive and negative solutions of a quasi-linear elliptic
equation by a mountain pass method and truncature techniques},
Nonlinear Anal, 59 (2004), 199--210.

\bibitem{GST} M. R. Grossinho, L. Sanchez and S. A. Tersian;
\emph{On the solvability of a boundary value problem for a fourth-order
ordinary differential equation, } Appl. Math. Letters   18 (2005),
439--444.

\bibitem{Jin} Z. Jin;
\emph{A truncation method for
semilinear elliptic equations}, Comm. P.D.E. 19 (1994), 605--616.

\bibitem{Lazer-Mckena2} A. C. Lazer and  P. J. McKenna;
 \emph{Global bifurcation and a theorem of Tarantello}, J.
Math. Anal. Appl. 181 (1994), 648--655.

\bibitem{Ma-Wang} R.Y. Ma  and H. Y. Wang;
\emph{On the existence of positive solutions of fourth-order
ordinary differential equation}, Appl. Anal. 59 (1995), 225--231.

\bibitem{Micheletti-Pistoia} A. M. Micheletti and A. Pistoia;
\emph{Multiplicity results for a fourth-order semilinear problem},
Nonlinear Anal. 31 (1998), 895--908.

\bibitem{Noussair} E.S. Noussair, C.A. Swanson and J.
Yang, \emph{Critical semilinear biharmonic equations in
$\mathbb{R}^N$}, Proc. Royal Soc. Edinburg 121A (1992), 139--148.

\bibitem{vivi} L. A. Peletier and V. Rottsch\"afer, \emph{ Pattern
selection of solutions of the Swift-Hohenberg equation}, Physica D
194 (2004), 95--126.

\bibitem{pevorst} L. A. Peletier and R. C. A. M. van der Vorst;
\emph{Existence and nonexistence of positive solutions of
nonlinear elliptic systems and biharmonic equation}, Differential
Integral Equations 5 (1992), 747--767.

\bibitem{qian-li} A. Qian and  S. Li;
\emph{On the existence of nontrivial solutions for a fourth-order semilinear
elliptic problem}, Abstr. Appl. Anal. (2005), no. 6, 673--683.

\bibitem{Berg}D. Smets and J.B. van den Berg;
\emph{Homoclinic solutions  for Swift-Hohenberg and
suspension bridge type equations}, J. Diff. Eqns. 184 (2002),
78--96.

\bibitem{Tarantello} G. Tarantello;
\emph{A note on a semilinear elliptic value problem},
Differential Integral Equations, 5 (1992) 561--565.

\bibitem{Tersian} S. Tersian and J. Chaparova;
\emph{Periodic and homoclinic solutions of extended
Fisher-Kolmogorov equations} J.
Math. Appl. Anal. 260(2001), 490--506.

\bibitem{Xavier} J. B. M. Xavier;
 \emph{Some existence theorems for equations of the form
$-\Delta u= f(x,u, Du)$}, Nonlinear
Anal. 15 (1990), 59--67.

\bibitem{Yan} Z. Yan;
 \emph{A note on the solvability in
$W^{2,p}(\Omega)$ for the equation $ -\Delta u= f(x,u, Du)$,}
Nonlinear Anal.  24 (1995), 1413--1416.

\end{thebibliography}

\end{document}
