\documentclass[reqno]{amsart}
\usepackage{hyperref}

\AtBeginDocument{{\noindent\small
\emph{Electronic Journal of Differential Equations},
Vol. 2009(2009), No. 75, pp. 1--8.\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{9mm}}

\begin{document}
\title[\hfilneg EJDE-2009/75\hfil Eigencurves for a steklov problem]
{Eigencurves for a Steklov problem}

\author[A. Anane, O. Chakrone, B. Karim, A. Zerouali\hfil EJDE-2009/75\hfilneg]
{Aomar Anane, Omar Chakrone, \\
Belhadj Karim, Abdellah Zerouali}  % in alphabetical order

\address{Universit\'e Mohamed I, Facult\'e des Sciences \\
  D\'epartement de Math\'ematiques et Informatique \\
  Oujda, Maroc}
\email[Aomar Anane]{ananeomar@yahoo.fr}
\email[Omar Chakrone]{chakrone@yahoo.fr}
\email[Belhadj Karim]{karembelf@hotmail.com}
\email[Abdellah Zerouali]{abdellahzerouali@yahoo.fr}

\thanks{Submitted March 3, 2009. Published June 5, 2009.}
\subjclass[2000]{35J70, 35P30}
\keywords{Principal eigencurve; Steklov problem;
$p$-Laplacian; \hfill\break\indent Sobolev trace embedding}

\begin{abstract}
 In this article, we study the existence of the eigencurves for
 a Steklov problem and we obtain their variational formulation.
 Also we prove the simplicity and the isolation results of each
 point of the principal eigencurve.  Also we obtain the continuity
 and the differentiability of the principal eigencurve.
\end{abstract}

\maketitle
\numberwithin{equation}{section}
\newtheorem{theorem}{Theorem}[section]
\newtheorem{lemma}[theorem]{Lemma}

\section{Introduction}

Consider the two parameter Steklov eigenvalue problem
 \begin{equation}
\begin{gathered}
\triangle_{p}u = 0    \quad \text{in }\Omega,\\
|\nabla u|^{p-2}\frac{\partial u}{\partial \nu}
= \lambda m(x)|u|^{p-2}u +\mu|u|^{p-2}u \quad  \text{on } \partial \Omega
 \end{gathered} \label{P1}
\end{equation}
where $ \Omega $ is a bounded domain in $\mathbb{R}^{N}$
$(N \geq 2)$ with a Lipschitz continuous boundary, $m \in
L^{\infty}(\partial\Omega)$ is a weight function which may change
sign, $\lambda, \mu, p$ be real numbers with
$1<p<\infty$. The weak solutions of \eqref{P1} are defined by
\begin{equation} \label{P2}
\int_{\Omega} |\nabla u|^{p-2}\nabla u \nabla \varphi \,dx = \lambda
\int_{\partial\Omega} m(x)|u|^{p-2}u \varphi \,d\sigma +
\mu\int_{\partial\Omega}|u|^{p-2}u \varphi \,d\sigma,
\end{equation}
for $\varphi\in W^{1, p}(\Omega)$,
where $\,d\sigma$ is the $N-1$ dimensional Hausdorff measure. Let us
note that all solutions of problem \eqref{P1} are of class
$C^{1, \alpha}(\Omega)$ since they are $p$-harmonic.


Problem \eqref{P1} has been studied  by several authors in the
case $\mu=0$ and $p=2$; we cite in particular the works
\cite{B,Es,S}. For the nonlinear case, the authors in \cite{AC2} and
\cite{T} studied the case when $\mu=0$ and $m\in
L^{q}(\partial\Omega)$. A problem in which the eigencurve appears in
the boundary condition has been considered recently in \cite{El}.
Assuming $m\in L^{\infty}(\partial\Omega)$ the authors show that for
each $\lambda \in \mathbb{R}$, there is
 an increasing  sequence of eigenvalues for the
 nonlinear boundary-value problem
 \begin{equation}
\begin{gathered}
\triangle_{p}u = |u|^{p-2}u   \quad \text{in }\Omega,\\
|\nabla u|^{p-2}\frac{\partial u}{\partial \nu} = \lambda
m(x)|u|^{p-2}u +\mu|u|^{p-2}u \quad   \text{on } \partial \Omega
 \end{gathered} \label{P3}
\end{equation}
also they show that the first eigenvalue is simple and isolated.
Furthermore they obtain some results about their variation, density,
and continuous dependence on the parameter $\lambda$.

We set
\begin{equation}
\begin{aligned}
\mu_{1}(\lambda)=\inf\Big\{&\frac{1}{p}\int_{\Omega}|\nabla
u|^{p}\,dx-\frac{\lambda}{p}\int_{\partial \Omega}m(x)|u|^{p}\,d\sigma:
u\in W^{1,p}(\Omega), \\
& \frac{1}{p}\int_{\partial
\Omega}|u|^p\,d\sigma=1\Big\},
\end{aligned} \label{e1.3}
\end{equation}
We understand by the principal eigencurve of the Steklov problem
\eqref{P1}, the graph of the map
$\mu_{1}:\lambda\to\mu_{1}(\lambda)$ from $\mathbb{R}$ to
$\mathbb{R}$.

Our purpose of this paper is to study , as in \cite{El}, the
existence of the eigencurves of the Steklov problem \eqref{P1} and
we obtain their variational formulation by using
Ljusternik-Schnirelmann theory (\cite{Sz}).
 Also we prove the simplicity and isolation results of each point of the principal
 eigencurve $\mu_{1}(\lambda)$ by applying Picone's Identity \cite{Al}. Finally, we obtain the continuity and the differentiability of this
principal eigencurve.

The plan of this paper is the following. In Section 2, we use a
variational method to prove the existence of a sequence of
eigencurves for the problem \eqref{P1}. In Section 3, we establish
 the simplicity and the isolation results of
each point of the principal eigencurve. Finally, in Section 4, we
establish the continuity of the eigenpair $(\mu_{1}(\lambda),
u(\lambda))$ in $\lambda$ and the differentiability of the principal
eigencurve.

\section{Existence of eigencurves}

To prove the existence of a sequence of eigencurves of
\eqref{P1}, we will use a variational approach and consider the
energy functional on $W^{1,p}(\Omega)$ as
$$
\Phi_{\lambda}(u)
=\frac{1}{p}\int_{\Omega}|\nabla u|^{p}\,dx - \frac{\lambda}{p}
\int_{\partial\Omega} m(x)|u|^{p}\,d\sigma,
$$
Set
$$
S:= \{u \in W^{1, p}(\Omega);
\frac{1}{p}\int_{\partial\Omega}|u|^{p}\,d\sigma = 1\}.
$$
 It is clear that for any $\lambda\in\mathbb{R}$, The solutions of
\eqref{P1} are the critical points  of $\Phi_{\lambda}$ restricted
to $S$. For any $k\in \mathbb{N}^*$, let
$$
\Gamma_{k}=\{K\subset S: K\text{ symmetric, compact and }
 \gamma(K)=k \},
$$
where $\gamma(K)=k$ is the genus of $K$; i.e., the smallest integer $k$
such that there is an odd continuous map from $K$ to
$\mathbb{R}^k\backslash\{0\}$. Next we define
\begin{equation} \label{e1.1}
\mu_{k}(\lambda):=\inf_{K\in \Gamma_{k}}\max_{u\in
K}\Phi_{\lambda}(u)
\end{equation}
and
$$
\|u\|:= \Big(\int_{\Omega}|\nabla u|^{p}\,dx +
\int_{\Omega}|u|^{p}\,dx\Big)^{1/p}
$$
is the $W^{1, p}(\Omega)$-norm.

The following theorem is the main result of this section.

\begin{theorem} \label{thm1}
For each $\lambda \in \mathbb{R}$, $\mu_{k}(\lambda)$ given by
\eqref{e1.1} is a nondecreasing sequence of positive eigenvalues of
the problem \eqref{P1}. Moreover $\mu_{k}(\lambda)\to
+\infty$ as $k \to +\infty$.
\end{theorem}

We will use Ljusternick-Schnirelmann theory on $C^1$-manifolds. It
is clear that for any $\lambda\in\mathbb{R}$, the functional
$\Phi_{\lambda}$ is even and bounded from below on $S$. Indeed, let
$u\in S$, then
\begin{equation}
\Phi_{\lambda}(u)\geq -|\lambda|\|m\|_{\infty,\partial
\Omega}>-\infty, \label{e3.1}
\end{equation}
where $\|\cdot\|_{\infty,\partial\Omega}$ denotes the
$L^{\infty}(\partial\Omega)$-norm. Letting
$$
A(u):= -\frac{\lambda}{p}\int_{\partial\Omega}m|u|^{p}\,d\sigma, \quad
B(u):= \frac{1}{p}\int_{\partial\Omega}|u|^{p}\,d\sigma.
$$
 By employing the Sobolev trace embedding
$W^{1,p}(\Omega)\hookrightarrow L^p(\partial \Omega)$,
 we deduce that $A$, $B$ are weakly continuous and $A'$, $B'$ are compact, where $A'$ and $B'$
 are respectively the derivative of $A$ and $B$.

We are now ready to prove the Palais-Smale condition.

\begin{lemma} \label{lem1}
 The functional $\Phi_{\lambda}$ satisfies the Palais-Smale
condition on $S$; i.e., for each sequence $(u_{n})_{n}\subset S$, if
$\Phi_{\lambda}(u_{n})$ is bounded and
\begin{equation}
(\Phi_{\lambda})'(u_{n})-c_{n}B'(u_n)\to 0, \label{e3.2}
\end{equation}
 with $c_n=\frac{\langle (\Phi_{\lambda})'(u_n),u_n\rangle}{\langle
B'(u_n),u_n\rangle}$. Then, $(u_n)_n$ has a convergent subsequence
in $W^{1,p}(\Omega)$.
\end{lemma}

Let define the property $(S_{+})$. We shall deal with operators $F$
acting from $W^{1,p}(\Omega)$ to $(W^{1,p}(\Omega))'$. $F$
satisfies the condition $(S_{+})$, if for any sequence $v_{n}$
weakly convergent to $v$ in $W^{1,p}(\Omega)$, and
$\limsup_{n\to +\infty}\langle F(v_{n}),
v_{n}-v\rangle \leq 0$ it follows that $v_{n}\to v$ strongly
in $W^{1,p}(\Omega)$, where $(W^{1,p}(\Omega))'$ is the dual of
$W^{1,p}(\Omega)$ with respect to the pairing $\langle ., .\rangle$.

\begin{proof}[Proof of Lemma \ref{lem1}]
Let us first show that the sequence $u_{n}$ is
bounded in $W^{1,p}(\Omega)$. Assume by contradiction that, for a
subsequence of $(u_{n})_{n}$, $\|u_{n}\| \to + \infty$ and
let $v_{n}:= u_{n}/\|u_{n}\|$, for a subsequence,
$v_{n}\to v$ weakly in $W^{1, p}(\Omega)$ and strongly in
$L^{p}(\Omega)$ and strongly in $L^{p}(\partial\Omega)$. Since
$\Phi_{\lambda}(u_{n})$ is bounded, then $\int_{\Omega}|\nabla
u_{n}|^{p}\,dx$ remains bounded, one has $\int_{\Omega}|\nabla
v_{n}|^{p}\,dx\to 0$. Thus $v$ is a nonzero constant, indeed;
the weak convergence of $v_{n}$ imply that
$$
\int_{\Omega}|\nabla v|^{p}\,dx+  \int_{\Omega}| v|^{p}\,dx \leq
\liminf_{n \to +\infty}\Big(\int_{\Omega}|\nabla
v_{n}|^{p}\,dx + \int_{\Omega}| v_{n}|^{p}\,dx\Big).
$$
Thus $\int_{\Omega}|\nabla v|^{p}\,dx = 0$, hence $v$ is a constant.
Moreover $v_{n}\to v$ strongly in $W^{1, p}(\Omega)$, thus
$v$ is a nonzero constant. But $B(u_{n}) = 1$ and so, dividing by
$\|u_{n}\|^{p}$ and passing to the limit, one obtains
$\int_{\partial\Omega}|v|^{p}\,d\sigma = 0$. This is a contradiction
(since $v$ is a nonzero constant). Thus $u_{n}$ is bounded in
 $W^{1,p}(\Omega)$. For a subsequence of $(u_{n})_{n}$,
 $u_{n}\to u$ weakly in
$W^{1,p}(\Omega)$ and strongly in $L^p(\partial\Omega)$. On the
other hand, by \eqref{e3.2}, $(\Phi_{\lambda})'(u_n)$ being a
convergent sequence strongly to some $f\in (W^{1,p}(\Omega))'$. By
calculation, we have
$$
\langle F(u_{n}), u_{n}-u\rangle = \langle (\Phi_{\lambda})'(u_{n}),
(u_{n}-u)\rangle - \langle A'(u_{n}), (u_{n}-u)\rangle +
\int_{\Omega}|u_{n}|^{p-2}u_{n}(u_{n}-u)\,dx, %\label{e3.3}
$$
 where $F$ is an operator defined
from $W^{1,p}(\Omega)$ to $(W^{1,p}(\Omega))'$ by
$$
\langle F(u), v\rangle =\int_{\Omega}|\nabla u|^{p-2}\nabla u\nabla
v \,dx+\int_{\Omega}|u|^{p-2}uv\,dx.
$$
Using the compactness of $A'$, we get
$$
\limsup_{n\to +\infty}\langle F(u_{n}),u_{n}-u\rangle \geq 0.
$$
Since the operator $F$ satisfies the condition $(S_{+})$, $u_{n}\to
u$ strongly in $W^{1,p}(\Omega)$. This achieves the proof of lemma.
\end{proof}

\begin{proof}[Proof of Theorem \ref{thm1}]
This theorem is proved by applying a general result from infinite
dimensional Ljusternik-Schnirelmann theory. We need only to prove
that for any $\lambda\in \mathbb{R}$, $\mu_{k}(\lambda)\to
+\infty$ as $k\to +\infty$. The proof adopts the scheme in
\cite{El}. Let $(e_{n},e_{j}^{*})_{n,j}$ be a biorthogonal system
such that $e_{n}\in W^{1,p}(\Omega)$, $e_{j}^{*}\in
(W^{1,p}(\Omega))'$, the $(e_{n})_{n}$ are dense in
$W^{1,p}(\Omega)$; and the $(e_{j}^*)_{j}$ are total in
$(W^{1,p}(\Omega))'$. Set for any $k\in \mathbb{N}^*$
$$
\mathcal{F}_{k-1}^{\bot}=\overline{\mathop{\rm span}
(e_{k+1},e_{k+2},e_{k+3},\dots)}.
$$
Observe that for any $K\in\Gamma_{k}$, $K\cap
\mathcal{F}_{k-1}^{\bot}\neq \emptyset$
(by \cite[(g) of Proposition 2.3]{Sz}). Now, we claim that
$$
t_{k}:=\inf_{K\in\Gamma_{k}}\sup_{K\cap\mathcal{F}_{k-1}^{\bot}}
\Phi_{\lambda}(u)\to +\infty, \quad \text{as } k\to +\infty.
$$
Indeed, to obtain the contradiction, assume for $k$ large enough
that there is $u_{k}\in \mathcal{F}_{k-1}^{\bot}$ with
$\frac{1}{p}\int_{\partial\Omega}|u_{k}|^p\,d\sigma=1$ such that
$$
t_{k}\leq \Phi_{\lambda}(u_{k})\leq M,
$$
for some $M>0$ independent of $k$. Therefore,
$$
\frac{1}{p}\int_{\Omega} |\nabla u_{k}|^p\,dx-
\frac{\lambda}{p}\int_{\partial\Omega} m(x)|u_{k}|^p\,d\sigma\leq M.
$$
Hence
\begin{equation}
\int_{\Omega} |\nabla u_{k}|^p\,dx\leq pM+
\lambda\|m\|_{\infty,\partial \Omega}< \infty. \label{e3.4}
\end{equation}
To prove that $(u_{k})_{k}$ is bounded in $W^{1,p}(\Omega)$, we
follow the same method in the proof of Lemma \ref{lem1}. Thus for a
subsequence of $(u_{k})_{k}$ if necessary, we can suppose that
$(u_{k})$ converges weakly in $W^{1,p}(\Omega)$ and strongly in
$L^p(\partial\Omega)$. By our choice of $\mathcal{F}_{k-1}^{\bot}$,
we have $u_{k}\to 0$ weakly in $W^{1,p}(\Omega)$. Because
$\langle e_{n}^{*},e_{k}\rangle = 0$, for all $k\geq n$. This
contradicts the fact that
$\frac{1}{p}\int_{\partial\Omega}|u_{k}|^{p}\,d\sigma=1$, for all $k$
and the the claim is proved.

Finally, since $\mu_{k}(\lambda)\geq t_{k}$ we conclude that
$\mu_{k}(\lambda)\to +\infty$, as $k\to+\infty$ and the proof is
complete.
\end{proof}


\section{Qualitative properties of the principal eigencurve}

Now we consider qualitative properties of the principal eigencurve .
Several authors studied the simplicity result in Dirichlet
$p$-Laplacian case by using $C^{1,\alpha}$-regularity and
$L^{\infty}$-estimation of the first eigenfunction, we cite in
particular  the works \cite{Al}, \cite{An} and \cite{Li}.

Let us note that all solutions of problem \eqref{P1} are of class
$C^{1, \alpha}(\Omega)$ since they are $p$-harmonic. Moreover,
following the procedure outlined in \cite{T2} one may show that all
solutions of problem \eqref{P1} belongs to $L^{\infty}(\Omega)$.

\begin{theorem} \label{thm4.1}
For any $\lambda\in\mathbb{R}$, the eigenvalue $\mu_{1}(\lambda)$
defined by \eqref{e1.3} is simple and the eigenfunctions
associated to $\mu_{1}(\lambda)$ are either positive or negative in
$\overline{\Omega}$.
\end{theorem}

The next lemma follows from Picone's identity.

\begin{lemma} \label{lem3.2}
Let $u$ and $v$ be two nonnegative eigenfunction associated to some
eigenvalues $\mu$ and $\tilde{\mu}$, respectively. Then
\begin{equation} \label{E} 0\leq (\mu -
\tilde{\mu})\int_{\partial\Omega}u^{p}\,d\sigma
\end{equation}
and equality holds if and only if $v$ is multiple of $u$.
\end{lemma}

\begin{proof}
We first show that the trace of $v$ satisfies $v>0$ on
$\partial\Omega$. Let $\epsilon > 0$. By the maximum principle of
Vazquez (see \cite{V}) $v>0$ in $\Omega$ so that $\frac{v}{v +
\epsilon} \to 1_{\Omega}$ in $L^{p}(\Omega)$ as $\epsilon
\to 0$. On the other hand $\nabla(\frac{v}{v + \epsilon})
\to 0$ a.e. as $\epsilon \to 0$. Taking $\varphi =
\frac{1}{(v + \epsilon)^{p-1}}$ as testing function in equation
\eqref{P2} satisfied by $v$, we have
$$
(p-1)\int_{\Omega}\frac{|\nabla v|^{p}}{(v + \epsilon)^{p}}\,dx =
\int_{\partial\Omega}(\lambda m + \mu)(\frac{v}{v +
\epsilon})^{p}\,d\sigma
$$
so that
$$
|\nabla(\frac{v}{v +
\epsilon})|^{p}= (\frac{\epsilon}{v + \epsilon})^{p}\frac{|\nabla
v|^{p}}{(v + \epsilon)^{p}}\leq \frac{|\nabla v|^{p}}{v^{p}}\in
L^{1}(\Omega).
$$
By the dominated convergence theorem, we have that
$\frac{v}{v + \epsilon} \to 1_{\Omega}$ in $W^{1,
p}(\Omega)$. By continuity of the trace mapping, we have that
$\frac{v}{v + \epsilon} \to 1_{\partial\Omega}$ in
$L^{1}(\partial\Omega)$ as $\epsilon \to 0$ and it follows
that $v>0$ on $\partial\Omega$. Now let $\epsilon>0$. By Picone's
identity, we have
\begin{align*}
0&\leq \int_{\Omega}|\nabla u|^{p}\,dx - \int_{\Omega}|\nabla
v|^{p-2}\nabla v \nabla(\frac{u^{p}}{(v + \epsilon)^{p-1}})\,dx \\
&= \int_{\partial\Omega}(\lambda m + \mu)u^{p}\,d\sigma -
\int_{\partial\Omega}(\lambda m + \tilde{\mu})(\frac{v}{v +
\epsilon})^{p-1}u^{p}\,d\sigma
\end{align*}
and equality holds if and only if $v$ is multiple of $u$. Going to
the limit $\epsilon\to 0$ and using the fact that $v>0$ on
$\partial\Omega$, we get the desired inequality.
\end{proof}

\begin{proof}[Proof of Theorem \ref{thm4.1}]
By Theorem \ref{thm1}, it is clear that $\mu_{1}(\lambda)$ is an
eigenvalue of the problem \eqref{P1} for any $\lambda\in\mathbb{R}$.
Let $u$ be an eigenfunction associated to $\mu_{1}(\lambda)$ so that
$|u|$ is a minimiser for \eqref{e1.3} and is thus an eigenfunction
associated to $\mu_{1}(\lambda)$. It follows from the maximum
principle of Vazquez that $|u|>0$ in $\Omega$ and we conclude that
$u$ has constant sign.

 Taking $\mu = \tilde{\mu} =
\mu_{1}(\lambda)$ in \eqref{E}, we see that any eigenfunction $v$
associated of $\mu_{1}(\lambda)$ must be a multiple of $u$, so that
$\mu_{1}(\lambda)$ is simple.
\end{proof}

To prove the isolation of $\mu_{1}(\lambda)$, we need the
following two lemmas.

\begin{lemma} \label{lem2}
Let $(k, q)\in\mathbb{N}^{*}\times\mathbb{N}$ and let
$\lambda\in\mathbb{R}$. If $\mu_{k}(\lambda)=
\mu_{k+1}(\lambda)=\dots =\mu_{k+q}(\lambda)$, then $\gamma(K)\geq q+1$
where
$$
K:=\{u\in S; u \mbox{ is an eigenfunction associated to
}\mu_{k}(\lambda)\}.
$$
\end{lemma}

The above lemma is proved by applying a general result from infinite
dimensional Ljusternik-Schnirelmann theory.


\begin{lemma} \label{lem3}
For each $\lambda\in\mathbb{R}$, $\mu_{1}(\lambda)$ is the only
positive eigenvalue associated with $\lambda$, having an
eigenfunction that does not change sign on the boundary
$\partial\Omega$.
\end{lemma}

\begin{proof}
For the proof, we use the Lemma \ref{lem3.2}. Taking
$\mu = \mu_{1}(\lambda)$ in \eqref{E}, we see that no eigenvalue
$\tilde{\mu}> \mu_{1}(\lambda)$ can be associated to a positive
eigenfunction. Thus $\mu_{1}(\lambda)$ is the only positive
eigenvalue associated to an eigenfunction of definite sign.
\end{proof}

\begin{theorem} \label{thm3.5}
For each $\lambda\in\mathbb{R}$, $\mu_{1}(\lambda)$ is isolated.
\end{theorem}

\begin{proof}
It suffices to prove that $\mu_{2}(\lambda)$ is indeed the second positive
eigenvalue of the problem \eqref{P1}, i.e.
$\mu_{1}(\lambda)<\mu_{2}(\lambda)$ for all $\lambda\in\mathbb{R}$
and if $\mu_{1}(\lambda)<\mu<\mu_{2}(\lambda)$, then $\mu$ is not an
eigenvalue of problem \eqref{P1}. By Theorem \ref{thm4.1},
$\gamma(K_{1})=1$ where $K_{1}:=\{u\in S; u \mbox{ is an
eigenfunction associated to }\mu_{1}(\lambda)\}$. Thus, by Lemma
\ref{lem2}, $\mu_{1}(\lambda)<\mu_{2}(\lambda)$.  By contradiction, we suppose
that $\mu$ is an eigenvalue of problem \eqref{P1}. Let $u$ be an
eigenfunction associated to $\mu$. Since $\mu \neq
\mu_{1}(\lambda)$, we deduce by Lemma \ref{lem3} that $u^{+}=
\max(u, 0)\neq 0$ and $u^{-}= \min(u, 0)\neq 0$. It follows from
\eqref{P2} that
\begin{gather*}
\int_{\Omega}|\nabla u^{+}|^{p}\,dx-
\lambda\int_{\partial\Omega} m(x)|u^{+}|^{p}\,d\sigma= \mu
\int_{\partial\Omega}|u^{+}|^{p}\,d\sigma,
\\
\int_{\Omega}|\nabla u^{-}|^{p}\,dx - \lambda\int_{\partial\Omega}
m(x)|u^{-}|^{p}\,d\sigma = \mu
\int_{\partial\Omega}|u^{-}|^{p}\,d\sigma
\end{gather*}
Assume that $u$ is normalized in such a way that
$$
\frac{1}{p}\int_{\partial\Omega}|u^{+}|^{p}\,d\sigma =
\frac{1}{p}\int_{\partial\Omega}|u^{-}|^{p}\,d\sigma=1.
$$
The set $K_{2}=\{\alpha u^{+}+ \beta u^{-}; \alpha, \beta \in\mathbf{R}
\mbox{ such that } |\alpha|^{p}+ |\beta|^{p}=1\}$ is in
$\Gamma_{2}$. Thus
\begin{align*}
\mu_{2}(\lambda)
&\leq \max_{|\alpha|^{p}+
|\beta|^{p}=1}\Big(\frac{1}{p}\int_{\Omega}|\nabla( \alpha
u^{+}+\beta u^{-})|^{p}\,dx -
\frac{\lambda}{p}\int_{\partial\Omega}m(x)|\alpha u^{+} + \beta
u^{-}|^{p}\,d\sigma\Big)\\
& = \mu.
\end{align*}
This is a contradiction. The proof of the isolation of
$\mu_{1}(\lambda)$ is complete.
\end{proof}

\section{Continuity and differentiability in $\lambda$}

In this section, we extend the results of continuity and
differentiability  for the first eigencurve of the Dirichlet
$p$-Laplacian shown by Binding and Huang in \cite{Bh}.

Let $\lambda\in\mathbb{R}$ and $(\mu_{1}(\lambda), u(\lambda))$
be the corresponding eigenpair. Henceforth we normalize the
eigenfunction $u(\lambda)$ to $u(\lambda)\in S$ with $u(\lambda)>0$.
In the following theorem, we consider continuity of the eigenpair in
$\lambda$ and differentiability of the principal eigencurve
$\mu_{1}(\lambda)$ in $\lambda$.

\begin{theorem} \label{thm4}
For any bounded domain $\Omega$,  the function $\lambda \to
\mu_{1}(\lambda)$ is differentiable on $\mathbb{R}$ and the function
$\lambda\to u(\lambda)$ is continuous from $\mathbb{R}$ to
$W^{1,p}(\Omega)$. More precisely
\begin{equation} \label{e4.0}
\mu_{1}'(\lambda_{0})=
-\frac{1}{p}\int_{\partial\Omega}m(x)(u(\lambda_{0}))^p\,d\sigma,\quad
\forall \lambda_{0} \in \mathbb{R}.
\end{equation}
\end{theorem}

\begin{proof}
By \eqref{e1.3}, it is easy to see that $\lambda \to
\mu_{1}(\lambda)$ is a concave function in $\mathbb{R}$. Continuity
of $\lambda \to \mu_{1}(\lambda)$ follows from the concavity.
To prove continuity of $\lambda\to u(\lambda)$, we proceed as
follows. Let $\Lambda\subset\mathbb{R}$ be bounded. For
$\lambda\in\Lambda$, since
$$
\mu_{1}(\lambda)=\frac{1}{p}\int_{\Omega}|\nabla u(\lambda)|^{p}\,dx
 -\frac{\lambda}{p}\int_{\partial\Omega}
m(x)|u(\lambda)|^{p}\,d\sigma \leq \text{constant},
$$
we have that $\int_{\Omega}|\nabla u(\lambda)|^{p}\,dx$ remains bounded.
To prove that $u(\lambda)$ is bounded in $W^{1,p}(\Omega)$,
we follow the same method in the proof of Lemma \ref{lem1}. Thus, for a
subsequence, $u(\lambda)\to u_{0}$ weakly in $W^{1,
p}(\Omega)$ and strongly in $L^{p}(\Omega)$ and strongly in
$L^{p}(\partial\Omega)$ as $\lambda \to \lambda_{0}\in
\overline{\Lambda}$. Passing to the limit in the following equality
\begin{equation} \label{e4.1}
\begin{aligned}
&\int_{\Omega} |\nabla u(\lambda)|^{p-2}\nabla u(\lambda) \nabla
\varphi \,dx\\
&= \lambda \int_{\partial\Omega} m(x)|u(\lambda)|^{p-2}u
\varphi \,d\sigma +
\mu_{1}(\lambda)\int_{\partial\Omega}|u(\lambda)|^{p-2}u(\lambda)
\varphi \,d\sigma,
\end{aligned}\end{equation}
we have
\begin{equation} \label{e4.2}
\begin{aligned}
&\int_{\Omega} |\nabla u_{0}|^{p-2}\nabla u_{0} \nabla \varphi \,dx \\
&= \lambda_{0} \int_{\partial\Omega} m(x)|u_{0}|^{p-2}u_{0} \varphi
\,d\sigma +
\mu_{1}(\lambda_{0})\int_{\partial\Omega}|u_{0}|^{p-2}u_{0} \varphi
\,d\sigma,
\end{aligned} \end{equation}
On the other hand $u_{0}\not\equiv 0$ (since $u_{0}\in S$). Thus
$u_{0}$ is an eigenfunction associated to $\mu_{1}(\lambda_{0})$. By
simplicity of $\mu_{1}(\lambda_{0})$, we have
$u_{0}=u(\lambda_{0})$. Taking $\varphi= u_{0}$ in \eqref{e4.2},
we obtain
\begin{equation} \label{e4.3}
\frac{1}{p}\int_{\Omega} |\nabla u_{0}|^{p}\,dx =
\frac{\lambda_{0}}{p} \int_{\partial\Omega} m(x)|u_{0}|^{p}\,d\sigma +
\mu_{1}(\lambda_{0}).
\end{equation}
For $\varphi= u(\lambda)$ in \eqref{e4.1}, we get
\begin{equation} \label{e4.4}
\frac{1}{p}\int_{\Omega} |\nabla u(\lambda)|^{p}\,dx =
\frac{\lambda}{p} \int_{\partial\Omega} m(x)|u(\lambda)|^{p}\,d\sigma
+ \mu_{1}(\lambda).
\end{equation}
Letting $\lambda \to \lambda_{0}$ in \eqref{e4.4}, we have
\[
\lim_{\lambda \to \lambda_{0}}
\frac{1}{p}\int_{\Omega} |\nabla u(\lambda)|^{p}\,dx
= \frac{\lambda_{0}}{p} \int_{\partial\Omega} m(x)|u_{0}|^{p}\,d\sigma +
\mu_{1}(\lambda_{0})
=\frac{1}{p}\int_{\Omega} |\nabla u_{0}|^{p}\,dx.
\]
Since $u(\lambda)\to u_{0}$ strongly in $L^{p}(\Omega)$,
$\|u(\lambda)\| \to \|u_{0}\|$ as $\lambda \to\lambda_{0}$.
Finally by the uniform convexity of $W^{1, p}(\Omega)$,
we conclude that $u(\lambda) \to u_{0}= u(\lambda_{0})$
strongly in $W^{1, p}(\Omega)$ as $\lambda
\to\lambda_{0}$.

For the differentiability of $\lambda \to \mu_{1}(\lambda)$, it
suffices to use the variational characterization of
$\mu_{1}(\lambda)$ and of $\mu_{1}(\lambda_{0})$, so that
$$
\frac{\lambda_{0}-\lambda}{p}\int_{\partial\Omega}m(x)(u(\lambda))^p
\,d\sigma
\leq \mu_{1}(\lambda)-\mu_{1}(\lambda_{0})
\leq \frac{\lambda_{0}-\lambda}{p}
 \int_{\partial\Omega}m(x)(u(\lambda_{0}))^p\,d\sigma,
$$
for all $\lambda,\lambda_{0}\in \mathbb{R}$. Dividing by $\lambda
-\lambda_{0}$ and letting $\lambda \to\lambda_{0}$, we
obtain \eqref{e4.0}.
\end{proof}

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