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\markboth{\hfil Four-parameter bifurcation \hfil EJDE--2001/06}
{EJDE--2001/06\hfil J. Fleckinger, R, Pardo, \& F. de Th\'elin \hfil}
\begin{document}
\title{\vspace{-1in}\parbox{\linewidth}{\footnotesize\noindent
{\sc  Electronic Journal of Differential Equations},
Vol. {\bf 2001}(2001), No. 06, pp. 1--15. \newline
ISSN: 1072-6691. URL: http://ejde.math.swt.edu or http://ejde.math.unt.edu
\newline ftp  ejde.math.swt.edu \quad ftp ejde.math.unt.edu (login: ftp)}
 \vspace{\bigskipamount} \\
 %
  Four-parameter bifurcation for a \\
  p-Laplacian system 
 %
\thanks{ {\em Mathematics Subject Classifications:} 
35J45, 35J55, 35J60, 35J65, 35J30, 35P30
\hfil\break\indent
{\em Key words:} p-Laplacian, bifurcation.
\hfil\break\indent
\copyright 2001 Southwest Texas State University. \hfil\break\indent
Submitted June 29, 2000. Published January 9, 2001. \hfil\break\indent
(R.P.) supported by grant PB96-0621 from the Spanish DGICYT } }
\date{}
%
\author{ Jacqueline Fleckinger, Rosa Pardo, \& Fran\c{c}ois de Th\'elin }
\maketitle

\begin{abstract} 
 We study a four-parameter bifurcation phenomenum arising in a
 system involving $p$-Laplacians: 
  $$\displaylines{ 
  -\Delta_p u = a \phi_p(u)+ b \phi_p(v) +  f(a , \phi_p (u), \phi_p (v)) ,\cr
  -\Delta_p v  =  c  \phi_p(u) + d \phi{p}(v)) + g(d , \phi_p (u), \phi_p (v)),
  }$$
 with $u=v=0$ on the boundary of a bounded and sufficiently smooth domain in
 $\mathbb{R}^N$; 
 here $\Delta_{p}u = {\rm div} (| \nabla u|^{p-2} \nabla u)$,
 with  $p>1$ and $p \neq 2$, is the $p$-Laplacian operator, and
 $\phi_{p} (s) =|s|^{p-2} s$ with  $p>1$. 
 We assume that  $a, b, c, d$ are real parameters. Thwn we 
 use a bifurcation method to exhibit some nontrivial solutions.
 The associated eigenvalue problem, with $f=g \equiv 0$, is also studied here.
\end{abstract}

% 
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\section{Introduction and Hypotheses}

We study some four-parameter bifurcation phenomena arising in the
system 
\begin{eqnarray} \label{p-System}
 &- \Delta_p u
 = a \phi_p(u)+ b \phi_p(v) + f(a , \phi_p (u), \phi_p (v)),&\nonumber \\
& - \Delta_p v  =  c  \phi_p(u) + d \phi{p}(v) + g(d 
, \phi_p (u), \phi_p (v)), \quad\mbox{in }\Omega & \\ 
&u  =  v = 0\,, \quad\mbox{on }\partial \Omega\,.& \nonumber
\end{eqnarray} 
where $ \Delta_pu = \mathop{\rm div} (| \nabla u|^{p-2} \nabla
u)$ for $p>1, \ p \neq 2$, is the $p$-Laplacian operator, $\phi_p 
:\mathbb{R}\to \mathbb{R}$ is given by $\phi_p (s) = |s|^{p-2} s, 
\ p>1$,  $\Omega \subset \mathbb{R}^{N}$ is a sufficiently smooth 
bounded domain,    and  $a, b ,c, d $ are real parameters. 

The operator $ {-\Delta}_p$ occurs in problems arising  in pure
mathematics, such as the theory of quasiregular and quasiconformal 
mappings (see \cite{To} and the references therein), and in 
a variety of applications, such as non-Newtonian fluids, 
reaction-diffusion problems, flow through porous media, nonlinear 
elasticity, glaciology, petroleum extraction, astronomy, etc (see 
\cite{At-EA,At-Ch,Di,Ar-Di}).  We also 
emphasize that systems such as (\ref{p-System}) are not easy 
generalizations of equations because the solutions cannot be 
obtained by variational methods. Here we use a bifurcation method 
to exhibit some nontrivial solutions. Another approach for non 
variational systems can be found in \cite{C-F-M-T}. Moreover the 
problem considered here where $p \neq 2$ is not a straightforward 
extension of the case $p=2$ due to the fact that the translations 
of the p-Laplacian are not always invertible neither commutative. 
 In this paper  we obtain bifurcation results for (\ref{p-System}).
The linear  case ($p=2$) is studied in \cite{F-P}.
The  case where $g\equiv 0$ is considered in \cite{F-M-T}.

We  assume through this article that the functions $f$ and $g$
satisfy the following Hypothesis:

A continuous function $f:\mathbb{R}^3 \to \mathbb{R}$ satisfies 
Hypothesis {\bf (H)} if there exists $\rho$ such that
$1 \leq \rho < {\frac{N+p'}{N-min(p,p')}}$ for  $\min (p,p')<N $
and $1 \leq \rho$ for $\min (p,p')\geq N$, and such that 
$$\displaylines{
\rlap{(H1)}\hfill 
\lim_{|(r,s)| \to 0} \frac{f(\lambda ,r,s)}{|(r,s)|}= 0\quad
\mbox{uniformly  with  respect to $\lambda$ on  bounded sets,} \cr
\rlap{(H2)} \hfill 
\lim_{|(r,s)|\to \infty} \frac{f(\lambda , r,s)}{|(r,s)|^{\rho}} = 0
\quad\mbox{uniformly  with  respect to $\lambda$ on  bounded sets.}
}$$ 
where, as usual, for a given $q>1$, $q'$ is defined by:
$$\frac{1}{q} + \frac{1}{q'}=1.$$


\paragraph{Definitions:}
By a solution of the system (\ref{p-System}) we mean a pair
$(A,(u,v))\in
 \mathbb{R}^4 \times (W_0^{1,p}(\Omega) )^2$, with 
$A:= \left(\begin{array}{cc} a & b \\ c & d\end{array}\right)$,  
satisfying (\ref{p-System}) in the
 weak sense, i.e., for all $w, z \in W_0^{1,p}(\Omega)$,
        \begin{eqnarray} \label{weak.p-System}
 \int _{\Omega} | \nabla
        u|^{p-2} \nabla u . \nabla  w & = & \int _{\Omega} a
        |u|^{p-2}u w + b |v|^{p-2}v w + f(a , \phi_p (u),
        \phi_p (v)) w \nonumber \\
 \int _{\Omega}| \nabla v|^{p-2}
        \nabla v .\nabla z & = & \int _{\Omega} c  |u|^{p-2}uz
         + d |v|^{p-2}v z + g(d , \phi_p (u), \phi_p (v)) z 
        \end{eqnarray} 
The set of solutions will be denoted by ${\cal
S}$.  Obviously $(A,(0,0))$ is a solution of (\ref{p-System}) for 
every $ (a ,b,c, d) \in \mathbb{R}^4$. The set of these pairs will 
be called the trivial solution set, and will be denoted by ${\cal 
S}_0$. 

We  say that $(A_0,(0,0)) \in {\cal S}_0$ is a {\em bifurcation
point} of (\ref{p-System}) with respect to the trivial solution
set iff every neighborhood of $(A_0,(0,0))$ contains solutions of
(\ref{p-System}) belonging to ${\cal S} \setminus {\cal S}_0$.

We will show that whenever (H) is satisfied, any matrix  $A_0$ 
with a negative eigenvalue, the other being the principal 
eigenvalue of the $p$-Laplacian, is such that $(A_0,(0,0)) \in 
{\cal S}_0$ is a  bifurcation point to positive solutions for 
(\ref{p-System}). 

To establish our results, we combine and adapt  methods of 
\cite{F-P} and \cite{F-M-T}.  Our paper is organized as follows: 
In Section 2, we recalls some results concerning the 
$p$-Laplacian. We recall in particular several lemmas established 
in \cite{F-M-T} concerning spaces that we will use. In Section 3, 
we show that if $(A_0,(0,0)) \in {\cal S}_0$ is a  bifurcation 
point, then the homogeneous system: $-\Delta_pU=A_0U$ has a non 
trivial solution. 
 In Section 4 we obtain conditions on $A_0$ for this to happen.
In Section 5 we compute the Leray-Schauder degree for the eigenvalue problem and
in Section 6
we state and establish our result.


\section{Notation and preliminaries}

In this section, we recall briefly some notation and results
concerning the p-Laplacian.

\noindent
{\bf The $p$-Laplacian},
$-\Delta_p$,  defined on $W_0^{1,p}(\Omega)$ has a first
eigenvalue $\lambda_1(p):=\lambda_1$ which is simple and isolated
\cite{An}; it is associated to a simple eigenfunction
$\varphi$ (normalized as $\|\varphi\|_{\infty}=1$) which is positive.
 Moreover, $\lambda_1$ is characterized by
      \begin{equation} \label{vp1}   
\lambda_1 = \inf_{u\in W^{1,p}_0; 
\int_{\Omega} |u|^p = 1}
    \int_{\Omega}\mid \nabla u\mid^p\,.
\end{equation}
The following results are known for the  equation 
 \begin{eqnarray} \label{p-Eq}
 &-\Delta_pu \, = \, k|u|^{p-2}u +f \quad\mbox{in } \Omega &\\
&u=0 \quad\mbox{on } \partial \Omega\,\label{cl}.&
 \end{eqnarray}
        
 \begin{lemma}[{\cite{V}}] \label{PM} 
 If $f\in L^{\infty}(\Omega)$, $f\geq 0$,
   $f\not \equiv 0$, Equation (\ref{p-Eq}-\ref{cl}) has at least one solution and
   satisfies the maximum principle
   (i.e. any solution $u$ is non-negative) if and only if $k<\lambda_1$.
\end{lemma}
        

\begin{lemma}[{\cite{F-G-T-T}}]
   For $f\in L^{\infty}$,
$f\geq 0$, $f\not \equiv 0$, and for $k=\lambda_1$, Equation
(\ref{p-Eq}-\ref{cl}) has no solution in $ W_0^{1,p}(\Omega)$.
\end{lemma}

\paragraph{The operator $T_q$.}
We introduce now some notation and results used in
\cite{F-M-T}. Let
\begin{equation}{\cal A}(q)= \left\{ \begin{array}{ll}
{\frac{Nq'}{N-min(q,q')}} &  \mbox{ if }   \min (q,q')<N \\
+\infty  &  \mbox{ if }     \min (q,q')\geq N
\end{array} \right.  \end{equation}
\begin{equation}{\cal B}(q)= \left\{\begin{array}{ll}
{\frac{Nq}{Nq -N+q}} &  \mbox{ if }    \min (q,q')<N \\ +1 &
\mbox{ if }    \min (q,q')\geq N.
\end{array} \right. \end{equation}
Then we  introduce the operator $ T_q:= -\Delta_q \circ
\phi_{q'}$ with domain
        $$ D(T_q) := \big\{ z \in L^{\alpha (q) }(\Omega) :
 \phi_{q'}(z) \in W_0^{1,p}(\Omega)\mbox{ and } -
 \Delta_q(\phi_{q'}(z)) \in  L^{\beta (q)} (\Omega) \big\}$$
Then
        $$\phi_q(W_0^{1,q})\hookrightarrow L^{\alpha}
        \hookrightarrow L^{\beta} \hookrightarrow
W^{-1,q'},$$ 
where $\alpha (q), \beta (q)$ are real numbers
satisfying $ {\cal B}(q) < \beta$, $\alpha < {\cal A}(q)$.

We notice that the operator $T_q$ is homogeneous of degree $1$.
 We also notice that the equation $ \ T_q u =
\lambda u \ $ has a solution $ \ u \not \equiv 0$, $u \in
W_0^{1,q}(\Omega)$ if and only if
 $ \ -\Delta_q u =
\lambda \phi_q(u) \ $ has a nontrivial solution. Such a
$\lambda$ is an eigenvalue and we denote by $ \ \sigma (-\Delta
_p) \ =  \ \sigma (T_p) \ $ these eigenvalues. If this solution is 
positive, then $\lambda=\lambda_1 $ and $u=k\varphi, \, k>0$. 

We have the following embeddings.

\begin{lemma}[{Lemma 2.2 in \cite{F-M-T}}]  If $\alpha < {\cal A}(q)$ the embedding
$\phi_q(W^{1,q})$ into $L^{\alpha}$ is compact. If $\beta > {\cal
B}(q)$, the embedding $L^{\beta}$ into $W^{-1,q'}$ is compact.
\end{lemma}
 
\begin{lemma}[{\cite{F-M-T}}]
 For $\alpha < {\cal A}(q)$, $\beta > {\cal B}(q)$, and $k<0$,
the operators $$T_q:D(T_q)\subset L^{\alpha} \longrightarrow
L^{\beta}\quad\mbox{and}\quad 
(T_q-k)^{-1}: L^{\beta} \longrightarrow L^{\alpha}$$
are well defined and $(T_q-k)^{-1}: L^{\beta} \longrightarrow
L^{\alpha}$ is completely continuous. 
\end{lemma}

\begin{lemma} {\it For $\alpha < {\cal A}(q)$, $\beta > {\cal B}(q)$,
 $k<\lambda_1$
 and $f\in L^{\beta}, f>0$,
$(T_q-k)^{-1}f$ is well defined or equivalently (\ref{p-Eq}) has a
unique solution.}\end{lemma}

\begin{remark} \rm
Obviously, $\Delta_q (-u)= -\Delta_q u$ and $\phi_q(-s)=
-\phi_q(s)$, then it follows that $T_q(-u)=-T_q(u)$ and by the previous Lemma 
with $k<\lambda_1$
 and $f\in L^{\beta}, f<0$,
$(T_q-k)^{-1}f$ is also well defined. When $f$ changes sign
several solutions may appear \cite{P-E-M,FHTT2}.
\end{remark}

\noindent
We also introduce
        $$ a(q)= \left\{ \begin{array}{ll}  \frac{Nq}{N-q} & \mbox{ if } 
        q<N \\ +\infty & \mbox{ if }  q\geq N.
        \end{array} \right.
        $$
From their definitions, it is easy to prove that, for any $q>1$, we have
        $$ (a(q))'<q' <  {\cal A}(q)\leq a(q'),$$
and that the functions $ (a(q))',  a(q')$ are decreasing in $q$.

\begin{lemma}
\label{imbedding} Assume that $ F: \mathbb{R}^3\to \mathbb{R}$ is 
continuous and satisfies {\rm (H)}. Choose $\alpha 
\in \mathbb{R}$ such that 
        $$ (a(p))'< \frac{\alpha }{\rho } < p' < \alpha < {\cal
        A}(p).$$
Then for any $ \lambda \in \mathbb{R}$ and for any $(w,z) \in L^{\alpha
}\times L^{\alpha }$, we have $F(\lambda ,w,z)\in L^{\beta }$,
where $\beta = \frac{\alpha }{\rho }$. Moreover, for any sequence
$\{ w_n ,z_n\}\in L^{\alpha }\times L^{\alpha }$, satisfying $(w_n
,z_n) \neq (0,0) $ and $\displaystyle \lim_{n\to \infty }
\| (w_n,z_n) \|_{L^{\alpha }\times L^{\alpha }}=0$, we have that
        $$ \limsup_{n\to \infty } \left\| \frac{F(\lambda ,w_n ,z_n )}{
\| (w_n,z_n) \|
        _{L^{\alpha }\times L^{\alpha } } } \right\| _{L^{\beta }}=0
        $$
\end{lemma}

\paragraph{Proof.} By (H) $\rho$ satisfies $1 \leq \rho <
{\frac{N+q'}{N-\min(q,q')}}$, if   $\min (q,q')<N $ and $1 \leq
\rho$ if $\min (q,q')\geq N$. It follows from Lemma 2.1 in
\cite{F-M-T} that we can choose $\alpha$ satisfying $$ (a(p))' <
\frac{\alpha }{\rho } < p' < \alpha < {\cal
        A}(p).$$
Moreover, for any $\delta >0$, there exists a constant $C$ such
that
        $$ |F(\lambda , r,s)| \leq \delta + C|(r,s)|^{\rho}, \quad
        \forall (r,s) \in \mathbb{R}\times \mathbb{R}\,;
        $$
hence the first assertion holds. Now, by H\"older‘ s inequality,
        \begin{eqnarray} \label{inequal}
\lefteqn{ \int _{\Omega } \Big| \frac{F(\lambda ,w_n ,z_n )}{ \|
(w_n,z_n) \|_{L^{\alpha }\times L^{\alpha } }} \Big|^{\beta } }\nonumber\\
&\leq& \Big( \int_{\Omega }
\big| \frac{F(\lambda ,w_n ,z_n )}{ | (w_n,z_n) |}
\big|^{\frac{\alpha }{\rho -1} }\Big)^{1/\rho'} 
\Big( \int _{\Omega }
\big| \frac{|(w_n ,z_n )|}{ \| (w_n,z_n) \|_{L^{\alpha } \times
L^{\alpha } }} \big|^{\alpha } \Big)^{1/\rho} \nonumber\\
&\leq& C_1 \Big( \int _{\Omega }
\big| \frac{F(\lambda ,w_n ,z_n )}{ | (w_n,z_n) |}
\big|^{\alpha/(\rho -1)}\Big)^{1/\rho'}.
\end{eqnarray}
From (H) we deduce
        $$
        \left| \frac{F(\lambda ,w_n ,z_n )}{ | (w_n,z_n) |}
\right|^{\frac{\alpha }{\rho -1} }
        \leq \delta ^{\frac{\alpha }{\rho -1}}+C_2 |(w_n ,z_n
        )|^{\alpha }.
        $$
Since $ \displaystyle \lim_{n\to \infty } \| (w_n,z_n)
\|_{L^{\alpha }\times L^{\alpha }}=0$,  for every $\delta >0$,
        $$ \limsup_{n\to \infty } \int _{\Omega } \left|
\frac{F(\lambda ,w_n ,z_n )
        }{ | (w_n,z_n) |} \right|^{\frac{\alpha }{\rho -1} }
        \leq \delta ^{\frac{\alpha }{\rho -1}} |\Omega |\,.
        $$
Taking into account (\ref{inequal}) the results follows. \hfill$\diamondsuit$

\section{Preliminary results}

In this section we show that if $(A_0,(0,0))$ is a bifurcation
point, then the eigenvalue problem 
\begin{eqnarray}\label{p-EP} 
&- \Delta_p u  =   a_0 \phi_p(u) + b_0 \phi_p(v), &\nonumber  \\ 
&- \Delta_p v  =  c_0  \phi_p(u) + d_0 \phi_p(v), \quad 
\mbox{in } \Omega    \\ 
&u = v = 0, \quad\mbox{on } \partial \Omega \,. \nonumber
\end{eqnarray} 
has a non-trivial solution.
This is well-known in the case $p=2$, (cf. \cite{C-R}), but due to
the nonlinearity of $T_p$, the proof is much more delicate.


\begin{theorem} \label{bif.p-EP}
Let $f,g$ satisfy $(H1)$, and $(A_0 , (0,0))$ be a bifurcation
point of (\ref{p-System}) in  $\mathbb{R}^4 \times 
(W_0^{1,p}(\Omega) )^2$ ; then the eigenvalue problem (\ref{p-EP}) 
has a non-trivial solution . 
\end{theorem}

\paragraph{Proof.} If $(A_0, (0,0))$ is a bifurcation point, then
there exists a sequence  \\ 
$\{(A_n, (u_{n},v_{n})) \}$ of nontrivial 
solutions of (\ref{p-System}), with  $A_n=(a_{n} , b_{n},c_{n}, 
d_n)\in \mathbb{R}^4$ and $ (u_{n},v_{n})\in 
(W_0^{1,p}(\Omega))^2$, such that 
$$
 A_{n}  \to A_0  \quad\mbox{in } \mathbb{R}^4 \quad\mbox{and}\quad
(u_{n},v_{n}) \to (0,0) \quad\mbox{in } (W_0^{1,p}(\Omega))^2.
$$
Define $w_{n} = \phi_p (u_{n}), \  z_{n}=
\phi_p(v_{n})$. Due to Lemma 2.2 (cf. \cite{F-M-T} ; Lemma 2.2), 
$w_{n}, \ z_{n} \in L^{\alpha}$ whenever $\alpha < {\cal A}(p)$. 
Moreover, $(A_{n} , (w_{n},z_{n}))$ is a nontrivial solution of
the system 
\begin{eqnarray} \label{p-TSystem}
 &T_p w_{n}  =   a_{n} w_{n} + b_{n} z_{n} + f(a_{n} ,
 w_{n}, z_{n} ) ,& \\ 
&T_p z_{n}  =  c_{n}  w_{n} + d_{n}
 z_{n} + g(d_{n} , w_{n} , z_{n} ) \quad\mbox{in }\Omega . & \nonumber
\end{eqnarray}
 Let $s_{n} = \max \{ \| w_{n}\|_{L^{\alpha}},
\| z_{n}\|_{L^{\alpha}} \}>0$. By Lemma 2.2 above
 it is obvious that $s_{n}
\to 0$ as $n \to \infty$. We  define
        $$ W_{n} = \frac{w_{n}}{s_{n}} , \quad Z_{n}=
\frac{z_{n}}{s_{n}}, \quad n \in \mathbb{N}
        $$ Dividing each equation of System (\ref{p-TSystem}) by
$s_{n}$ we can write 
\begin{eqnarray}
  &W_{n}  =   T_p^{-1}\left( a_{n} W_{n} + b_{n} Z_{n} +
  \frac{1}{s_{n}} f(a_{n} , w_{n}, z_{n} ) \right) ,&\nonumber \\
  &Z_{n}  =  T_p^{-1} \left(c_{n}  W_{n} + d_{n} Z_{n} +
  \frac{1}{s_{n}} g(d_{n} , w_{n} , z_{n} ) \right), \nonumber
\quad\mbox{in } \Omega\,.& 
\end{eqnarray}
From Lemma \ref{imbedding},
$ f(\mathbb{R}\times L^{\alpha} \times L^{\alpha} ) \subset
L^{\beta}$ for $\beta = \frac{\alpha}{\rho}$ and
        $$ \limsup_{n \to \infty} \left\| \frac{f(a_{n} ,
w_{n}, z_{n} )}{s_n} \right\|_{L^{\beta}} = 0.
        $$
        Of course an analogous result holds for $g$. Therefore,
$$
a_{n} W_{n} + b_{n} Z_{n} + \frac{1}{s_{n}}f(a_{n} , w_{n}, z_{n} )
\quad\mbox{and}\quad
 c_{n}  W_{n} + d_{n} Z_{n} + \frac{1}{s_{n}} g(d_{n} ,
w_{n} , z_{n})
$$
are bounded sequences in $L^{\beta}$ with $\beta <\alpha $.
It follows from the compactness $T_p^{-1} : L^{\beta} \to 
L^{\alpha}$ that there exists two convergent subsequences 
        $$\displaylines{
 T_p^{-1} \Big( a_{n} W_{n} + b_{n} Z_{n} +
\frac{1}{s_{n}} f(a_{n} , w_{n}, z_{n} ) \Big) \to W\,,\cr
 T_p^{-1} \Big( c_{n}  W_{n} + d_{n} Z_{n} +
\frac{1}{s_{n}} g(d_{n} , w_{n} , z_{n}) \Big) \to Z
}$$
 in $L^{\alpha}$ and $(W,Z) \neq (0,0)$. Moreover
$(W_{n},Z_{n}) \to (W,Z)$ in $L^{\alpha}$ and
\begin{eqnarray} 
&T_p  W  =  a_0 W + b_0 Z,&\nonumber \\
&T_p Z  =  c_0  W + d_0 Z, \quad\mbox{in }\Omega ,& \nonumber
\end{eqnarray}
or equivalently, $(W,Z)$ is a nontrivial solution of the
eigenvalue problem (\ref{p-EP}).


\section{An Eigenvalue problem}

In this section we  consider the eigenvalue problem (\ref{p-EP})
with
 $(a_0 , b_0,c_0, d_0)=(a ,b,c, d)$. We establish
 necessary and sufficient conditions so that System $(3.1)$ has a
nontrivial positive solution.

\paragraph{Definition.} We say that $A =  \left( \begin{array}{c c} a &
 b \\ c & d \end{array} \right)$ satisfies the {\it solvability 
condition}, and we write $A\in {\cal S}(T_p)$, if there exists a 
nontrivial  solution of
 \begin{equation} \label{p-TP}
 T_p \left( \begin{array}{c} w
        \\ z \end{array} \right) = A \left( \begin{array}{c} w \\ z
        \end{array} \right)\,,
 \end{equation}
where   $ \ w:= \phi_p (u)$, $z=\phi_p(v)$, $w, z \in D(T_p)$ 
with 
        $$ D(T_p) := \{ z \in L^{\alpha (p) }(\Omega):
         \phi_{p'}(z) \in W_0^{1,p}(\Omega), \;
       -\Delta_p(\phi_{p'}(z)) \in  L^{\beta (p)} (\Omega)\},   
$$
and $\alpha (p), \beta (p)$ satisfy
        \begin{equation}
({\cal B}(p))'< \beta (p) \leq \alpha (p) < {\cal A}(p) .
        \end{equation}
We remark that Problem $(3.1)$ is equivalent to the  operator
equation (\ref{p-TP}).

\paragraph{Definition.} Let $\sigma(A)$ denote the spectrum of the
 Matrix $A$. Let ${\cal M}^-$ be the set of matrices that have a 
negative eigenvalue.

\begin{remark} \rm
Since $A$ has real coefficients the eigenvalues
are complex conjugate; and if  one is real,  both eigenvalues
are real. The eigenvalues, denoted by $\gamma$ and $\delta$, 
are the roots of the equation
\begin{equation} \label{eq2} X^2 -(a+d)X +ad-bc=0.
\end{equation}
If the eigenvalues are not real, $\gamma = \xi + i \eta$ and 
$\delta = \xi - i \eta$; therefore, $\gamma \delta= \xi^2 + 
\eta^2 >0$. since $\gamma\delta=ad-bc$, complex values occur only  
when $ad-bc>0$. 
\end{remark}

When $A$ in ${\cal M}^-$, we denote by $\gamma$ the negative eigenvalue.

\begin{proposicion} \label{(C)}
\begin{description}
\item[(a)]
 If $ \sigma(T_p) \cap \sigma (A)$ is not empty,
then $A$ is in ${\cal S}(T_p)$. More precisely, let $\lambda$ be 
in $\sigma (T_p) \cap \sigma (A) $, let $D\in \mathbb{R}^2$ be its 
corresponding $A$-eigenvector, let $\phi \in D(T_p)$  be its 
corresponding $T_p$-eigenfunction, then $D\phi$ solves (4.1). 
Consequently, if $\lambda_1 \in \sigma(A)$, and either 
$b(\lambda_1 -a)>0, \ (\geq 0)$ or $c(\lambda_1 -d)>0, \ (\geq 0)$  
the eigenvalue problem $(4.1)$ has a positive (nonnegative) 
solution. 
\item[(b)] Conversely, if $A \in {\cal M}^- \cap {\cal S}(T_p)$, then
$ \sigma (T_p) \cap \sigma (A) $  is not empty.
 Moreover if
 $A \in {\cal M}^-$ and if the eigenvalue problem $(4.1)$ has a positive
solution,
 then $ \sigma (T_p) \cap \sigma (A) = \{\lambda_1\}.$
\end{description}
\end{proposicion}

This proposition can also be stated as follows:\\
(a) If one of the eigenvalues of $A$ is in $\sigma(T_p)$ then there
exists a nontrivial   solution of  (\ref {p-TP}).\\
(b) Conversely, if $A$ has a negative eigenvalue,
and if there exists a nontrivial  solution of  (\ref {p-TP}),
then the other eigenvalue of $A$ is in $\sigma (T_p) $.

\begin{remark}
 In part (b) above, if $\sigma(A) := \{\gamma, \delta \}$
and if $\gamma<0$, necessarily
$\delta>0$, and  we have $\gamma \delta =ad-bc<0$.
 \end{remark}


\paragraph{Proof of Proposition (\ref{(C)})}

{\bf (a)} Assume that  $\lambda \in \sigma (A) \cap \sigma(T_p)$. By
definition of $\lambda$,
 there exists an eigenfunction $\varphi \in D(T_p), \ \varphi $ such that
 $T_p \varphi = \lambda \varphi$.
 Since  $\lambda \in \sigma (A)
\subset \mathbb{R}$,
  there exists an eigenvector
 $D= \left( \begin{array}{l} d_1 \\ d_{2} \end{array} \right) \in
\mathbb{R}^2$ such that $AD= \lambda D$. Define $(\eta, \zeta):= 
(d_1 \varphi, d_{2} \varphi) $. Since $T_p$ is homogeneous of 
order 1, 
        $$
T_p \left( \begin{array}{c} \eta \\ \zeta \end{array} \right)  
= T_p D \varphi = D T_p \varphi =
 \lambda D \varphi = A D \varphi = A  \left( \begin{array}{c} \eta
\\ \zeta \end{array} \right) 
$$
i.e. $(\eta, \zeta)$ is a  nontrivial  solution of (\ref{p-TP}),
and $ (d_1 \phi_{p'} (\varphi), d_{2} \phi_{p'}(\varphi)) \neq 
(0,0)$ is a  nontrivial solution of
(\ref{p-EP}).  Moreover, if $\lambda=\lambda_1$, we can take $\varphi>0$, 
and either
$(w,z)= (|b|,|\lambda_1 -a|)\phi$ or $(w,z)=(|c|,|\lambda_1 -d|)\phi$ 
is a positive (nonnegative) solution (or $b=c=0, a=d=\lambda_1$ and 
$(1,0)\phi, \ (0,1)\phi$ are
nonnegative solutions).

{\bf (b)} Let $(w,z) \neq (0,0)$ be a  nontrivial solution of (\ref{p-TP}),
i.e. $(w,z)$ is a  nontrivial  solution of
\begin{eqnarray} \label{syst}
&T_pw=aw+bz& \nonumber\\ 
&T_pz=cw+dz& \\
&w=z=0 \quad\mbox{on }\partial \Omega\,.&\nonumber
\end{eqnarray} We first consider some obvious cases.

 If $w=0$, then $z\not = 0$ satisfies $T_p z= d z$, therefore $d\in
\sigma(T_p)$ and $(T_p - a I)w= b z$ implies $b=0;$ consequently
$d \in \sigma (A)$ is an eigenvalue of $A$ and of $T_p$. Likewise,
$z=0$ implies that $a\in \sigma (A)$ is an eigenvalue of $A$.
Hence we assume now that $w\neq 0, \ z\neq 0.$

 If $b=0$, then $T_p w= a w$ with $w\neq 0$, implies that $a \in
\sigma (A) \cap \sigma(T_p)$. On the same way,  $c=0$ implies that
$d\in \sigma (A) \cap \sigma(T_p)$. Hence we assume now that $bc
\neq 0$.

 Now $bc\neq 0, $  and assume that $\gamma$ is a
negative eigenvalue of $A$. Moreover let us assume that  $w\neq 0,
\ z\neq 0$ are solutions of (\ref{p-TP}).

 System (\ref{p-TP}) can also be written as
        \begin{equation} \label{sistemagamma}
(T_p -\gamma I) \left( \begin{array}{c} w
        \\ z \end{array} \right) = \left( \begin{array}{c c} a
        -\gamma & b \\ c & d -\gamma \end{array} \right) \left(
        \begin{array}{c} w \\ z \end{array} \right).
 \end{equation}
Moreover, since $\gamma \in \sigma (A)$, it satisfies
        \begin{equation}
        \label{determinante}
        (a - \gamma )(d - \gamma) = bc.
        \end{equation}

From the first equation in  (\ref{syst}),
we obtain $(T_p - a I)w= b z$ with $z\in D(T_p)$. 
Applying  $(T_p - \gamma I)$ on both sides of this equation,
 and taking into account the second equation in
(\ref{syst}) we obtain: 
$$ (T_p -\gamma I)(T_p - a I)w = (T_p 
        -\gamma I)bz =  bcw + b(d - \gamma) z.$$
Taking into account  ( \ref{determinante}) and
(\ref{sistemagamma}) we derive
        \begin{equation} \label{Tp-eigenvalues}
        (T_p -\gamma I)(T_p - a I)w =
         (d - \gamma ) [ (a - \gamma) w +bz] =
         (T_p -\gamma I)(d - \gamma)w .
        \end{equation}
We observe that, in order to obtain the previous relations, we use
the homogeneity of $T_p$ but we cannot commute $T_p-\gamma I$ and
$T_p-aI$ because of the non linearity of $T_p$.

Since $\gamma  <0$, $(T_p-\gamma I)^{-1}$ is well defined,
applying it into (\ref{Tp-eigenvalues})  we obtain: $(T_p - a I)w 
=(d - \gamma)w $, or equivalently $$T_p w \, = \, ( a + d - 
\gamma)w $$ so that $a+d-\gamma$ is an eigenvalue of $T_p$. 
Since the eigenvalues of $A$ are real and equal to
\begin{equation} ( a+d)/2  \pm \sqrt{((a-d)/2)^2+bc}, \end{equation}
if $\gamma<0$ is an eigenvalue of $A$, the other is
 $\delta=a+d-\gamma$.
  Moreover, if  $w>0$, $z>0$, $T_p w \, = \, \delta w $ implies
  $\delta=\lambda_1$.


\section{The Leray-Schauder degree for the eigenvalue problem}


In this section we study the Leray-Schauder degree
 in terms of the Jordan canonical form of  matrices $A \in {\cal M}^-$. 
For this purpose we  use the following property:
If $A \in {\cal M}^-$
 and $\sigma (A) \cap \sigma (T_p) = \emptyset$ then 
$A \notin {\cal S}(T_p)$.
Therefore $(\ref{p-TP})$ has only the trivial
solution, which comes from Proposition \ref{(C)}.(b).


We denote by  $\ \sigma (A ) = \{ \gamma, \delta \} \ $  the
spectrum of Matrix $A$ , and $ \ \sigma (-\Delta _p) \ =  \ \sigma 
(T_p) \ $ the set of eigenvalues of the operator $ \ -\Delta_p \ $ 
with Dirichlet boundary conditions. 

\begin{proposicion}
\label{deg-LS}
 Let ${\cal U }\subset  (L^{\beta (p)}(\Omega))^2$ be open  bounded and 
$0 \in \cal U$. Let $J$
be the Jordan canonical form of the matrix $A $. Assume that $A 
\in {\cal M}^-$ and $\sigma (A) \cap \sigma (-\Delta_p ) = 
\emptyset $. Then 
        $$ \deg_{LS} ( I -  T_p ^{-1} A, {\cal U} , 0) = \deg_{LS} ( I -
T_p^{-1} J, {\cal U }, 0).
        $$
Moreover, one of the following two conditions is satisfied
\begin{enumerate}
\item   $ J =\left( \begin{array}{c c}\gamma & 0 \\ 0 &
\delta   \end{array} \right)$
and
$\deg_{LS} ( I -  T_p^{-1} J, {\cal U} , 0)$\\
$=\deg_{LS} (
I - \gamma T_p^{-1} , {\cal U} \cap L^{\beta (p) }(\Omega), 0)
  \deg_{LS} ( I - \delta T_p^{-1} , {\cal U} \cap L^{\beta (p)
}(\Omega) , 0)$ 
\item $J =\left( \begin{array}{c c}\gamma & 0 \\ 1 & \gamma\end{array}\right)$
and \\
$ \deg_{LS} ( I - T_p^{-1} J, {\cal U} , 0)= [ \deg_{LS} ( I -
 \gamma T_p^{-1} , {\cal U }\cap L^{\beta (p) }(\Omega), 0)]^2.
$
\end{enumerate}
\end{proposicion}

\begin{remark} \rm This result has been obtained for $p=2$ in
\cite[Proposition 2.1]{F-P}. In this case, the Leray-Schauder
degree for compact linear operators applies \cite{De,L-S}).

For $p\neq 2$, the question of calculating
$\deg_{LS} (I-\gamma T_p^{-1},{\cal U} \cap L^{\beta (p) }(\Omega), 0)$
has been answered in the following cases
\begin{itemize}
\item When the spatial dimension $N=1$ \cite{G-V,P-E-M}.
\item With radial symmetry  \cite{An2,P-M}.
\item Whenever $\gamma <\lambda_1$ or $\lambda_1<\gamma <\lambda_2$
\cite{An,P-M}).
\end{itemize}
The other cases are still open problems.
We consider here the case $\gamma<0<\lambda_1$.
\end{remark}

\paragraph{Proof of Proposition \ref{deg-LS}} 
Let $P$ be the invertible matrix such that
$A=P^{-1}JP$. Let $M_{2\times 2}(\mathbb{R})$ be the space of 
$2\times 2$-matrix with real coefficients. Let us consider a 
continuous function 
$ { \cal P } : [0,1] \to  M_{2\times 2}(\mathbb{R})$ such that:
1)  ${ \cal P } (t)^{-1}$ exists for all $ t \in [0,1]$,
2) ${ \cal P } (0) =I$, and 3) ${ \cal P } (1) = P$.

 Let us now define the homotopy
$ h:[0,1] \times ( L^{\beta (p) }(\Omega))^2 \to
        (L^{\alpha (p) }(\Omega))^2 $ by
        $$ h \left( t, \left( \begin{array}{c} w \\ z  \end{array}
        \right) \right) = T_p^{-1} \left[ { \cal P } (t)^{-1}J { \cal P }
(t)\right]
 \left( \begin{array}{c} w \\ z \end{array} \right),
        $$
        so that
        $$ h \left( 0, \left( \begin{array}{c} w \\ z      \end{array}
        \right) \right) = T_p^{-1} J  \left( \begin{array}{c} w
\\ z       \end{array} \right),  \quad 
        h \left( 1, \left( \begin{array}{c} w \\ z      \end{array}
        \right) \right) = T_p^{-1}A \left( \begin{array}{c} w \\ z
 \end{array} \right)
        $$
         If there exists some nontrivial solution of
          $$  h \left( t, \left( \begin{array}{c} w \\ z
\end{array} \right) \right) =          \left( \begin{array}{c} w
\\ z  ,       \end{array} \right) $$
then $\left[ { \cal P } (t)^{-1}J { \cal P }
(t)\right] \in {\cal S}(T_p)$ which is impossible by Proposition
\ref{(C)}, since $ \sigma \left[ { \cal P } (t)^{-1}J { \cal P }
(t)\right] =\sigma(J)
 = \sigma(A)$, $A\in {\cal M}^-$ and
$\sigma(T_p) \cap \sigma \left[ { \cal P } (t)^{-1}J { \cal P }
(t)\right] = \emptyset$. So   $  h \big( t, \big(
\begin{array}{c} w \\ z
\end{array} \big) \big) \neq         \big( \begin{array}{c} w
\\ z         \end{array} \big) $
 for any  $  \big( \begin{array}{c}
w \\ z      \end{array} \big) \neq  \big( \begin{array}{c} 0
\\ 0        \end{array} \big)$.

Now the invariance property for homotopies of the Leray-Schauder
degree proves that
        $$ \deg_{LS} ( I - T_p^{-1} A, { \cal U } , 0) = \deg_{LS} ( I -
T_p^{-1} J, { \cal U } , 0),
        $$ with $A=P^{-1}JP.$

We consider separately the following two cases:\\
{\bf Case $(i)$:}
 By the product formulae \cite[Theorem 8.5]{De}, and since
$\gamma, \delta \notin \sigma (-\Delta_p)$, we have
$$ 
\deg_{LS} ( I-T_p^{-1} J, { \cal U } , 0) =  \deg_{LS}
( (I - \gamma T_p^{-1},I) , { \cal U } , 0)  \deg_{LS} ( (I, I -
\delta T_p^{-1}) , K  , 0) 
$$
 where $(I - \gamma T_p^{-1},I) (w,z) = ((I -
\gamma T_p^{-1})w,z) $ and $K$ is the connected component of  $ \  
L^{\beta (p) }(\Omega)^2 \setminus ( I - T_p^{-1} J)(\partial { 
\cal U } )$ containing  zero. The reduction property states that 
        $$ \deg_{LS} ( (I - \gamma T_p^{-1},I) , { \cal U } , 0)
=\deg_{LS} ( I - \gamma T_p^{-1} , { \cal U } \cap L^{\beta (p)
}(\Omega), 0)
        $$ and Part $(i)$ is proved.
\\
{\bf Case (ii):}
$ J = \left( \begin{array}{c c}\gamma & 0 \\ 1 & \gamma
\end{array} \right)$.
Here $ \sigma (A) = \{ \gamma, \, \gamma<0 \} $ and $A$
is a non-diagonalizable matrix.

Let us define the homotopy $H:[0,1] \times ( L^{\beta
(p)}(\Omega))^2 \to ( L^{\alpha (p)}(\Omega))^2 $ by
        $$ H \left( t, \left( \begin{array}{c} w \\ z      \end{array}
\right) \right) = (T_p)^{-1} \left( \begin{array}{c c}\gamma & 0
\\ t & \gamma       \end{array} \right)
 \left( \begin{array}{c} w \\ z \end{array} \right).
        $$
We have $\sigma \left( \begin{array}{c c}\gamma & 0 \\ t & \gamma
\end{array} \right) = \sigma \left( \begin{array}{c c}\gamma & 0 \\ 0 &
\gamma  \end{array} \right) = \sigma (A) $. By Proposition
\ref{(C)}, and due to $A\in {\cal M}^-$, if $H(t,.)$ has a
non-trivial solution then $ \sigma \left( \begin{array}{c c}\gamma
& 0 \\ t & \gamma
\end{array} \right) \cap \sigma (-\Delta _p ) \neq \emptyset,$
which contradicts the hypothesis $ \sigma (A) \cap \sigma (-\Delta
_p) = \emptyset . $ Therefore
        $ \deg_{LS} ( I - H(t,.), {\cal U } , 0) $ is well defined and
independent of $t\in [0,1]$. Moreover by using again the product
formulae
\begin{eqnarray*}
 \deg_{LS} ( I - (T_p)^{-1} J, {\cal U} , 0) 
& = & \deg_{LS} ( I - H(1,.), {\cal U }, 0) \\ 
& = & \deg_{LS} (I - H(0,.), {\cal U }, 0) \\ 
& = & [\deg_{LS} ( I - \gamma
        (T_p)^{-1} , {\cal U }\cap  L^{\beta (p)}(\Omega) , 0)]^2.
\end{eqnarray*}


\section{Existence of Positive Bifurcated Solutions}

In this section we study sufficient conditions for the existence
of positive solutions bifurcating from  $(A_0 , (0,0) )$ where
$A_0= \left(
\begin{array}{cc} a_0 & b_0 \\ c_0 & d_0 \end{array}
\right)$. From Theorem~\ref{bif.p-EP}
 we will need that the eigenvalue problem has a (nontrivial)
 non negative solution, and therefore we will require,
 from Proposition \ref{(C)},
that $\lambda_1 \in \sigma ( A_0)$ and therefore $\sigma(T_p) \cap 
\sigma ( A_0) \not= \emptyset$. Another usual requirement is that 
 there is a changement of topological degree
(cf. \cite{Ra},\cite[Theorem 28.1]{De}, \cite{A-A}, ...). More explicitly, we have the
following

\begin{theorem}
Assume that $f,g$ satisfy (H), that $\lambda_1 \in \sigma (
A_0)$
  and that $A_0 \in \cal M.$
Then $(A_0 , (0,0) )$ is a bifurcation point to positive solutions
of (\ref{p-System}) in $\mathbb{R}^4 \times (W_0^{1,p}(\Omega) )^2$. 

Moreover, there is a connected component of topological dimension
$\geq 4$ of the set of nontrivial solutions of (\ref{p-System}) in
$\mathbb{R}^4 \times (W_0^{1,p}(\Omega) )^2$ whose closure 
contains the point $(A_0, (0,0))$. 
\end{theorem}

\begin{remark} \rm
 Theorem above is a generalization for systems of the already known 
situation for one single equation \cite[Proposition 2.2]{P-M}.
\end{remark}

\paragraph{Proof.} Hereafter we denote by $B_E(c,r)$ the ball in some 
space $E$ with center $c \in E$ and radius $r$. Suppose that  
$(A_0 , (0,0) )$ is not a bifurcation point of (\ref{p-System}). 
Since $\lambda_1$ is isolated, there are $\epsilon_0 >0$ and   
$r_0>0$ such that for every 
$A \in B_{\mathbb{R}^4}( A_0, \epsilon_0) \subset \mathbb{R}^4 \quad $, 
if $(w,z) \in B_{(W_0^{1,p})^2}((0,0), r_0) \subset (W_0^{1,p})^2$ 
satisfies (\ref{p-System}), then $(w,z)=(0,0)$. 

Since for any $A \in B_{\mathbb{R}^4}( A_0 , \epsilon_0)$
 the functions 
        $$ f(a , .,.) , \  g(d ,.,.) : (L^{\alpha})^2
\to L^{\beta }
        $$
 map bounded sets into bounded sets, the function
$ F: B_{\mathbb{R}^4}( A_0 , \epsilon_0 )
\times (L^{\alpha})^2 \to (L^{\alpha})^2$ given by
        $$ F \left( A , \left( \begin{array}{c} w
        \\ z   \end{array} \right) \right) = T_p^{-1} \left[ \left(
\begin{array}{c c}a & b \\ c & d  \end{array} \right)
 \left( \begin{array}{c} w \\ z \end{array} \right) +  \left(
 \begin{array}{c}  f(a , w,z)  \\  g(d ,w,z)       \end{array}
 \right) \right]
        $$ 
is completely continuous, consequently
$ \deg_{LS} ( I - F(A,.), B_{(L^{\alpha})^2} ((0,0), r_0),0)$ 
is well defined and independent of 
$A\in B_{\mathbb{R}^4}( A_0 , \epsilon_0 )$.
%
For  $A_0= \left( \begin{array}{c c} a_0 & b_0
\\ c_0 & d_0 \end{array} \right)$, denote by $J_0$ its Jordan
canonical form. By hypothesis we can always choose two matrices,
$A_i=  \left( \begin{array}{c c}a_i & b_i
\\ c_i & d_i      \end{array} \right)$, $i=1,2$, such that
        \begin{enumerate}
\item[(a)]  $\sigma (A_i) \cap  \sigma
(-\Delta_p) = \emptyset ,$
\item[(b)]   $A_i \in \cal M$
\item[(c)] $ A_i \in  B_{\mathbb{R}^4}(
A_0 , \epsilon_0 ) $ and
\item[(d)] $    \deg_{LS} ( I -  T_p ^{-1} A_1, { \cal U } , 0) \neq
\deg_{LS} ( I - T_p^{-1} A_{2}, { \cal U } , 0).$
        \end{enumerate}
 Let us now define the homotopies
        $$ H_i \left( t, \left( \begin{array}{c} w \\ z  \end{array}
        \right) \right) = T_p^{-1} \left[ A_i
 \left( \begin{array}{c} w \\ z \end{array} \right) + t  \left(
 \begin{array}{c}  f(a , w,z)  \\  g(d ,w,z)     \end{array}
 \right) \right],
        $$ Next, we  show by contradiction
that there exists a real number  sufficiently small again denoted
by $r_0$ such that
        $$ H_i \left( t, \left( \begin{array}{c} w \\ z  \end{array}
        \right) \right) \neq \left( \begin{array}{c} w \\ z \end{array}
        \right) \quad
         \mbox{in}  \quad \partial  B_{(L^{\alpha})^2}((0,0), r_0) \subset
         (L^{\alpha})^2 $$ for any $t\in [0,1]$.
Assume that for any $n\in \mathbb{N}$ large enough, there exists a
sequence
        $$ \left\{  \left( t_{n} , \left( \begin{array}{c} w_{n}
\\ z_{n}  \end{array} \right) \right) \right\} \in [0,1] \times
(L^{\beta})^2, \ \ \ \left\|  \left( \begin{array}{c} w_{n}
\\ z_{n}   \end{array} \right) \right\|_{(L^{\beta})^2} = 1/n ,
        $$ and
        $$ T_p  \left( \begin{array}{c} w_{n} \\ z_{n}   \end{array}
\right) =
 A _i \left( \begin{array}{c} w_{n} \\ z_{n}  \end{array} \right) +
 t_{n}  \left( \begin{array}{c}  f(a , w_{n},z_{n})  \\  g(d
 ,w_{n},z_{n})    \end{array} \right) , \quad\mbox{in }\Omega,
        $$ $$ w_{n}=z_{n}=0, \quad\mbox{on }\partial \Omega.
        $$ Arguing as in the proof of Theorem (\ref{bif.p-EP}), the
associated eigenvalue problem has a non-trivial solution
 which is positive. Hence, by Proposition (\ref{(C)}),
        $$\lambda_1 \in  \sigma (A_i) \cap
\sigma (-\Delta_p)  $$ which contradicts  (a). Then $H_i 
(t, (w,z)) \neq (w,z) $ in $ \partial B_{(L^{\alpha})^2}((0,0), 
r_0 ) $, therefore $ \deg_{LS} ( I - H_i(t,.), B_{(L^{\alpha})^2} 
((0,0), r_0),0)$ is well defined and independent of $t$, 
consequently 
\begin{eqnarray*}
\lefteqn{ \deg_{LS} ( I - F(A_i , .
        ), B_{(L^{\alpha})^2} ((0,0), r_0),0)}\\
&=&\deg_{LS} ( I - H_i(1,.), B_{(L^{\alpha})^2} ((0,0), r_0),0) \\ 
& = & \deg_{LS} ( I - H_i(0,.),
B_{(L^{\alpha})} ((0,0), r_0),0) \\ 
& = & \deg_{LS} ( I - T_p ^{-1} A_i,  B_{(L^{\alpha})^2} ((0,0), r_0) , 0)
\end{eqnarray*} 
which, jointly with (c) and (d), contradicts the assertion
that \\
$ \deg_{LS} ( I - F(A_i ,.),
  B_{(L^{\alpha})^2} ((0,0), r_0),0)$ is constant for
   $  A\in  B_{\mathbb{R}^4}( A_0 , \epsilon_0 ) $.

Now, we  built the nonnegative the matrices $A_1, A_2$. 
>From the definition of the Jordan's canonical form, there exists an 
invertible matrix $P$  such that $A_0=P^{-1}J_0P$. 
Denote now by $\gamma<0$ and $\delta$ 
the eigenvalues of $A$. Assume that $\delta = \lambda_1$. Let us 
define 
$$ A_1:= P^{-1} \left( \begin{array}{cc} \delta +\epsilon
& 0 \\ 0 & \gamma \end{array} \right) P , \quad A_{2}:=
P^{-1} \left( \begin{array}{cc} \delta -\epsilon & 0 \\ 0 & \gamma
\end{array} \right) P .
        $$
Now, the fact that
$ T_p ^{-1} : (L^{\beta})^2 \to (W^{1,p}_0)^2$
is continuous ensures that $ (A_0,(0,0)) $ is a bifurcation point of
(\ref{p-System}). The change of the degree and the Theorem of
Alexander and Antman \cite{A-A} complete the present proof.


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\end{thebibliography}

\noindent{\sc Jacqueline Fleckinger}  \\
{\sc CEREMATH \& UMR MIP}, Universit\'{e} Toulouse 1 \\ 
pl. A. France\\ 
31042 Toulouse Cedex, France \\
e-mail: jfleck@univ-tlse1.fr
\smallskip

\noindent{\sc Rosa Pardo} \\
Departamento de Matem\'atica Aplicada  \\ 
Universidad Complutense de Madrid \\ 
Madrid 28040, Spain \\
e-mail: rpardo@sunma4.mat.ucm.es \smallskip

\noindent{\sc Fran\c{c}ois de Th\'elin}\\ 
{\sc UMR MIP},  Universit\'{e} Toulouse 3 \\ 
118 route de Narbonne\\ 
31062 Toulouse Cedex 04, France \\
e-mail: dethelin@mip.ups-tlse.fr


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