\documentclass[reqno]{amsart}
\usepackage{hyperref}
\usepackage{esint}

\AtBeginDocument{{\noindent\small
\emph{Electronic Journal of Differential Equations},
Vol. 2012 (2012), No. 223, pp. 1--18.\newline
ISSN: 1072-6691. URL: http://ejde.math.txstate.edu or http://ejde.math.unt.edu
\newline ftp ejde.math.txstate.edu}
\thanks{\copyright 2012 Texas State University - San Marcos.}
\vspace{9mm}}

\begin{document}
\title[\hfilneg EJDE-2012/223\hfil Stability of positive steady-state solutions]
{Stability of positive stationary solutions to a spatially heterogeneous
 cooperative system with cross-diffusion}

\author[W.-T. Li, Y.-X. Wang, J.-F. Zhang \hfil EJDE-2012/223\hfilneg]
{Wan-Tong Li, Yu-Xia Wang, Jia-Fang Zhang}  % in alphabetical order

\address{Wan-Tong Li \newline
School of Mathematics and Statistics, Lanzhou University\\
Lanzhou, Gansu 730000, China}
\email{wtli@lzu.edu.cn}

\address{Yu-Xia Wang \newline
School of Mathematics and Statistics, Lanzhou University\\
Lanzhou, Gansu 730000, China}
\email{wangyux10@163.com}

\address{Jia-Fang Zhang \newline
School of Mathematics and Information Sciences, Henan University \\
Kaifeng, Henan 475001,  China}
\email{jfzhang@henu.edu.cn}

\thanks{Submitted October 10, 2012. Published December 4, 2012.}
\subjclass[2000]{35K57, 35R20, 92D25}
\keywords{Cross-diffusion; heterogeneous environment;
stability; \hfill\break\indent Hopf bifurcation; steady-state solution}

\begin{abstract}
 In the previous article [Y.-X. Wang and W.-T. Li, J.
 Differential Equations, 251 (2011) 1670-1695], the authors have
 shown that the set of positive stationary solutions of a
 cross-diffusive Lotka-Volterra cooperative system can form an
 unbounded fish-hook shaped branch $\Gamma_p$. In the present paper,
 we will show some criteria for the stability of positive stationary
 solutions on $\Gamma_p$. Our results assert that if $d_1/d_2$ is
 small enough, then unstable positive stationary solutions bifurcate
 from semitrivial solutions, the stability changes only at every
 turning point of $\Gamma_p$ and no Hopf bifurcation occurs. While as
 $d_1/d_2$ becomes large, the stability has a drastic change when
 $\mu<0$ in the supercritical case. Original stable positive
 stationary solutions at certain point may lose their stability, and
 Hopf bifurcation can occur. These results are very different from
 those of the spatially homogeneous case.
\end{abstract}

\maketitle
\numberwithin{equation}{section}
\newtheorem{theorem}{Theorem}[section]
\newtheorem{lemma}[theorem]{Lemma}
\newtheorem{definition}[theorem]{Definition}
\newtheorem{proposition}[theorem]{Proposition}
\newtheorem{remark}[theorem]{Remark}
\allowdisplaybreaks

\section{Introduction}


It is known that the spatial heterogeneity has an important impact
on the population dynamics besides the interactions between species
\cite{add1,add2,add3,add4,add5,hu,add8,add9,add90,add10}.
Cross-diffusion has also been shown to produce richer
stationary patterns by many researchers, see
\cite{add6,add7,kuto2,kuto,kuto1,LiWang,lou,add12,add13,add14,
wang,wang1,wang2,wang3,wang4,Zeng1,Zeng2,add15,wu1,caofu,zhangfu}
and references therein. In this paper, we study the following
Lotka-Volterra cooperative system with cross-diffusion in a
spatially heterogeneous environment:
\begin{equation}
 \begin{gathered}
 u_{t}=d_{1}\Delta u+u(a_1-b_1 u+c_1(x)v), \quad  x\in \Omega, t>0,\\
 v_{t}=\Delta[(d_2+\rho(x)u)v] +v(a_2-b_2 v+c_2(x)u), \quad
 x\in \Omega, t>0,\\
 \partial _{\nu}u=\partial _{\nu} v=0, \quad
 x\in \partial \Omega, t>0,\\
 u(x,0)=u_{0}(x)\geq 0,\quad v(x,0)=v_{0}(x)\geq 0,
 \quad
 x\in \bar{\Omega}.
 \end{gathered} \label{00}
 \end{equation}
Here $\Omega$ is a bounded domain in $\mathbb{R}^{N}$ ($N\geq 1$)
with smooth boundary $\partial \Omega$; $\nu$ is the outward unit
normal vector on $\partial \Omega$ and
$\partial_{\nu}={\partial}/{\partial \nu}$; $u(x,t)$ and $v(x,t)$ represent
the population densities of the two species interacting and
migrating in the same habitat $\Omega$; $a_1$ and $a_2$, which are
real constants and may be negative, denote the birth or death rates
of the respective species; positive constants $b_1$ and $b_2$
represent the intra-specific pressures of $u$ and $v$; the
inter-specific pressures $c_1(x)$ and $c_2(x)$ with $c_1(x),
c_2(x)\geq \not\equiv 0$ are assumed to be spatially heterogeneous
and continuous in $\bar{\Omega}$; positive constants $d_1$ and $d_2$
represent the natural dispersive forces of movements of the species,
respectively; $\rho(x)$ is a smooth positive function in
$\bar{\Omega}$ with $\partial_\nu \rho(x) |_{\partial
\Omega}=0$. Furthermore, the system is self-contained, and there is
no flux on $\partial \Omega$.


The nonlinear diffusion term
$$
\Delta(\rho(x)uv)= \nabla \cdot [\rho(x)u \nabla v+v \nabla (\rho(x)u)]
$$
is usually referred as the cross-diffusion term.  This is first
proposed by  Shigesada et al. \cite{shigesada} to model the
segregation phenomenon of two species. The diffusion term here means
that the diffusive direction of $v$ is affected not only by the
population pressure of $u$ but also the heterogeneity of the
environment, which implies that $v$ diffuses to the low
density region of $\rho(x)u$. See \cite{okubo} for more ecological
backgrounds.

By a simple scaling
$$(\lambda, \mu, k, b(x), d(x), \tilde{u}, \tilde{v})
=\Big(\frac{a_1}{d_1}, \frac{a_2}{d_2},
 \frac{d_1}{d_2b_1},\frac{d_2}{d_1b_2}c_1(x),
 \frac{d_1}{d_2b_1}c_2(x),\frac{b_1}{d_1}u,\frac{b_2}{d_2}v \Big),
$$
system \eqref{00} is reduced to the  coupled system
\begin{equation}
\begin{gathered}
 d_1^{-1}u_{t}=\Delta u+u(\lambda- u+b(x)v), \quad x\in \Omega, t>0,\\
 d_2^{-1}v_{t}=\Delta[(1+k\rho(x)u)v] +v(\mu- v+d(x)u), \quad
 x\in \Omega, t>0,\\
 \partial _{\nu}u=\partial _{\nu} v=0, \quad x\in \partial \Omega, t>0,\\
 u(x,0)=\bar{u}_{0}(x)\geq 0,\quad v(x,0)=\bar{v}_{0}(x)\geq 0,
 \quad x\in \bar{\Omega}.
 \end{gathered} \label{01}
 \end{equation}
For simplicity, we have dropped the `` $\tilde{}$ " sign in
\eqref{01}. Local solvability of \eqref{01} has been established by
Amann \cite{add2}, whereas the global solvability is very difficult
and needs a careful and further study. In the paper, we are mainly
interested in the dynamical behavior of nonnegative solutions to
\eqref{01}. Clearly, the corresponding stationary
problem of \eqref{01} is
\begin{equation}
\begin{gathered}
 \Delta u+u(\lambda-u +b(x)v)=0,
 \quad  x\in \Omega,\\
 \Delta [(1+k\rho(x)u) v]+v(\mu-v+d(x)u)=0, \quad  x\in \Omega, \\
 \partial _{\nu}u=\partial _{\nu} v=0, \quad x\in \partial \Omega.
 \end{gathered} \label{02}
 \end{equation}


In a previous article \cite{wang}, the authors have obtained the
global bifurcation branch of positive solutions of \eqref{02} under
weak cooperation ($\|b\|_{\infty}\|d\|_{\infty}<
\frac{\min_{\bar{\Omega}}}{\rho/\|\rho\|_{\infty}}$) and large
cross-diffusion effect, where $(u, v)$ is said to be a positive
solution of \eqref{02} if $u>0$ and $v>0$ in $\bar{\Omega}$. So a
positive solution $(u, v)$ means a coexistence state of the two
interacting species.  We expect that the bifurcation curve
$\Gamma_p$ can  not only yield multiple positive stationary
solutions but also show us much more complicated spatio-temporal
patterns of \eqref{01}. Since it is very difficult to obtain the
complete structure of the solution set of \eqref{02} and many
problems still remain open now, our main attention is focused on the
stability analysis of the positive stationary solutions and large
time behaviors of \eqref{01} under weak cooperation.

For the stability of positive stationary solutions to
cross-diffusion systems, Kan-on \cite{kan} has given some criteria
on the stability of nonconstant stationary solutions to
a singular perturbed type competition model proposed by Mimura et
al. \cite{mimura}. In 2004, Kuto \cite{kuto1} considered a
cross-diffusion system arising in a prey-predator population model.
By the method of linearization principle for quasilinear
parabolic equations developed by Potier-Ferry \cite{ferry}, he
investigated the asymptotic stability of positive stationary
solutions obtained by him and Yamada \cite{kuto2}. Furthermore, he
showed that Hopf bifurcation phenomenon could occur on the
positive stationary solution branch under some
conditions. However, the coefficients in the prey-predator
population model are all spatially homogeneous. Recently, he
\cite{kuto} further considered the predator-prey population model in
a spatially heterogeneous environment and established the stability
and Hopf bifurcation of positive stationary solutions obtained in
\cite{kuto3} by  similar methods. Motivated by \cite{kuto1,kuto},
the aim of this paper is to establish some criteria for the
stability of positive stationary solutions of the Lotka-Volterra
cooperative model \eqref{01} by our existence results
\cite{wang}.

Our first result is concerned with the case that the diffusive ratio
$d_1/d_2$ is small enough, in which case the stability
of all positive stationary solutions on the bifurcation continuum
can be determined clearly. To be precise, unstable
positive stationary solutions bifurcate from semitrivial solutions,
and the stability changes only at every critical point of the
bifurcation curve with respect to the bifurcation parameter
$\lambda$, and no Hopf bifurcation occurs. Moreover, different from
\cite{kuto1} and \cite{kuto}, we can further determine that the
number of the critical points is odd. From the above
stability result, we see that although the spatial heterogeneity has
an ability to produce multiple positive stationary solutions, while
it does not have a strongly beneficial effect on the species in low
densities. Furthermore, if the bifurcation at the semitrivial
solution is supercritical (the bifurcation curve is no longer
$\subset$-shaped), then stable positive stationary solutions
bifurcate from semitrivial solutions, and the number of critical
points is even. On the contrary, if the diffusive ratio $d_1/d_2$ is
sufficiently large, the stability result totally changes, which is
our second result. At this time, we only show that the spatial
segregation of $\rho(x)$ and $b(x)$ and small $\|b\|_{\infty}$ can
produce Hopf bifurcation at certain point on $\Gamma_p$ if $\mu<0$.
More precisely, if the bifurcation direction is
supercritical, in which case both $(0,0)$ and $(\lambda, 0)$ are
unstable near the bifurcation point, as $d_1/d_2$ varies
from a small number to a large one, stable positive stationary
solutions bifurcate from the semitrivial solution for small
$d_1/d_2$, and some stable positive stationary solutions will lose
their stability and Hopf bifurcation occurs near the bifurcation
point for large $d_1/d_2$. Therefore, time periodic solutions are
obtained for problem \eqref{01} near the Hopf bifurcation point.
Whereas, two Hopf bifurcation points can be found for the
predator-prey system \cite{kuto}.

If the coefficients are spatially homogeneous, then the situation is
rather different. As pointed out in \cite{wang}, we know that under
weak cooperation and constant coefficients, the corresponding
cooperative system with large cross-diffusion coefficient $k$ has a
unique positive stationary solution if $\lambda\in (\lambda^*,
\infty)$ and no positive stationary solutions if $\lambda\leq
\lambda^*$ in case $\mu>0$. If $\mu<0$, $\lambda^*$ should be
replaced by $\lambda_*$. Furthermore, our results imply that the
unique positive stationary solution is asymptotic stable,
nondegenerate, and Hopf bifurcation can never appear regardless of
the values of the natural diffusive rates $d_1$ and $d_2$. Thus, if
the environment is spatially heterogeneous, there exist much more
complicated dynamical behaviors for the weakly cooperative system,
including the change of the stability of some positive stationary
solutions and the appearing of Hopf bifurcation.


Finally, we point out that there is a common point for the
predator-prey and cooperative system under either Neumann or
Dirichlet boundary condition. That is, if one species has a large
cross-diffusion rate, and the interacting species has a rather small
natural diffusion rate comparing to the species, then the stability
changes at every turning point of the bifurcation curve;
while if the interacting species has a relatively large
natural diffusion rate, then Hopf bifurcation can occur. Thus, one
sees that the diffusion has a stronger effect on the stability of
positive stationary solutions than the boundary
condition, while the boundary condition can have an important effect
on the existence of positive stationary solutions as pointed out in
\cite{wang}.


The organization of this paper is as follows: In Section 2, we show
the global positive stationary bifurcation branch $\Gamma_p$ of
\eqref{01} obtained in \cite{wang}. The main results including the
asymptotic stability and Hopf bifurcation are stated in
Section 3. Finally, the proofs of asymptotic stability and Hopf
bifurcation are given in Sections 4 and 5,
respectively.

In  this article, the usual norm of $C(\bar{\Omega})$ is
defined by $\|u\|_{\infty}=\max_{\bar{\Omega}}| u(x)|$. Moreover, we
denote the average of $f(x)$ over $\Omega$ by 
$\fint_{\Omega} f(x)= \frac{1}{|\Omega|}\int_{\Omega} f dx$ and let $\lambda_1(q)$
represent the principal eigenvalue of the problem
 $$-\Delta u+q(x)u=\lambda u \quad {\rm{in}} \quad \Omega,
\quad  \quad \partial_\nu u=0 \quad {\rm{on}}\quad \partial
\Omega,$$
 for a continuous function $q(x)$.


\section{Preliminary Results}


In this section, we give the bifurcation structure of positive
stationary solutions of \eqref{01}. One can refer to \cite{wang}
for details.

In this paper, we work in  the following Sobolev spaces
\begin{equation*}
 X=W_\nu^{2,p}(\Omega)\times W_\nu^{2,p}(\Omega),\quad 
 Y=L^p(\Omega)\times L^p(\Omega), p>N,
 \end{equation*}
where $W_\nu^{2,p}(\Omega)=\{u\in W^{2,p}(\Omega): \partial_\nu
u =0 ~\rm{on} ~\partial \Omega\}$.

Set
\begin{equation}\label{32}
u=\varepsilon w,\quad (1+k \rho(x)u)v=\varepsilon z,\quad
\lambda=\varepsilon \alpha, \quad \mu=\varepsilon \beta, \quad
k=\frac{1}{\varepsilon},
\end{equation}
where $\varepsilon>0$ is a small constant,  $\alpha$ and $\beta$ are
real numbers. Then \eqref{01} is equivalent to the following system
\begin{equation}
\begin{gathered}
 d_1^{-1}w_{t}=\Delta w+\varepsilon F(w, z, \alpha), \quad x\in \Omega, t>0,\\
 d_2^{-1}\big[-\frac{\rho(x)z}{(1+\rho(x)w)^2}w_t+\frac{z_t}{1+\rho(x)w}\big]
 =\Delta z  +\varepsilon G(w, z), \quad  x\in \Omega, t>0,\\
 \partial _{\nu}w=\partial _{\nu} z=0, \quad  x\in \partial \Omega, t>0,\\
 w(x,0)=u_{0}/\varepsilon,\quad z(x,0)=(1+\rho(x)w_0)v_0/\varepsilon,
 \quad  x\in \bar{\Omega},
 \end{gathered} \label{33}
 \end{equation}
 where
\begin{gather*}
 F(w, z, \alpha)=w\Big(\alpha- w+\frac{b(x)z}{1+\rho(x)w}\Big),\\
 G(w, z)=\frac{ z}{1+\rho(x)w}\Big(\beta- \frac{z}{1+\rho(x)w}+d(x)w\Big).
 \end{gather*}
By defining $H: X\to Y$ and $B: X \times \mathbb{R}\to Y $ as
\begin{equation*}
H(w, z)=(\Delta w, \Delta z),\quad
B(w, z, \alpha)=\left(F(w, z, \alpha), G(w, z)\right),
\end{equation*}
 the positive stationary solution problem
 associated with \eqref{33} becomes
\begin{equation}\label{37}
H(w, z)+\varepsilon B(w, z, \alpha)={\bf{0}}.
\end{equation}
Let $P: X\to X_1$ and $Q: Y\to Y_1$ be the
orthogonal projections, where $X_1$ and $Y_1$ represent  the
$L^2-$orthogonal complements
 of $\mathbb{R}^{2}$ in $X$ and $Y$, respectively. Then the Lyapunov-Schmidt reduction
 asserts the following lemma.

\begin{lemma}\label{lemma3.1} 
For any $C>0$, there exist a small positive number $\varepsilon_0$
and a neighborhood
$N_0$ of $\left\{(w, z, \alpha, \varepsilon)=(r, s, \alpha, 0)\in X
\times \mathbb{R}^{2}: |r|, |s|, |\alpha|\leq C \right\}$ such that
the function $(w, z, \alpha, \varepsilon)$ is a positive solution of \eqref{37}
contained in $N_0$ if and only if
$$
(w, z, \alpha, \varepsilon)=\left((r, s)+\varepsilon {\bf{U}}(r, s, \alpha,
\varepsilon), \alpha, \varepsilon\right)
$$
and
$$
\Phi^\varepsilon(r, s, \alpha)=(I-Q)B\left((r, s)
+\varepsilon {\bf{U}}(r, s, \alpha, \varepsilon), \alpha \right)={\bf{0}}.
$$
\end{lemma}


 In the extreme case $\varepsilon=0$, we know that
\begin{equation*}
\Phi^0(r, s, \alpha)
=\begin{pmatrix} r\left(\alpha-r+s\fint_{\Omega}\frac{b(x)}{1+r\rho(x)} \right)\\
s\left(\fint_{\Omega}\frac{1}{1+r\rho(x)}\left(\beta-\frac{s}{1+r\rho(x)}+rd(x)
\right) \right)
\end{pmatrix}.
\end{equation*}
Then $\mathcal{L}_p=\{(r, f(r), g(r)): r\in \mathbb{R}
\}\subseteq{\mathcal {N}} (\Phi^0)$, where
\begin{equation}\label{310}
f(r)=\fint_{\Omega}\frac{\beta+rd(x)}{1+r\rho(x)}\bigg
/\fint_{\Omega}\frac{1}{(1+r\rho(x))^2}, \quad
g(r)=r-f(r)\fint_{\Omega}\frac{b(x)}{1+r\rho(x)}.
\end{equation}

In fact, $\mathcal{L}_p$ yields a limiting set of positive solutions
of \eqref{37}. More precisely, we have the following two
propositions.

\begin{proposition}\label{thm3.2}
Assume $\beta>0$,
$\|b\|_{\infty}\|d\|_{\infty}<\frac{\min_{\bar{\Omega}}\rho}{\|\rho\|_{\infty}}$.
Then for a sufficiently large $A>0$, there exist a small constant
$\varepsilon_1>0$ and a family of bounded smooth curves
\begin{equation}\label{71}
 \{S(\xi, \varepsilon)=(r(\xi, \varepsilon), s(\xi, \varepsilon),
 \alpha(\xi, \varepsilon)) \in \mathbb{R}^{3}: (\xi, \varepsilon) \in
 [0, C_\varepsilon]\times [0, \varepsilon_1]\}
 \end{equation}
such that for any $\varepsilon\in(0, \varepsilon_1]$, all positive
solutions of \eqref{37} with $\alpha \in [-c\beta
\|b\|_{\infty}, A ]$ can be expressed by
\begin{equation} \label{72}
\begin{aligned}
\Gamma^{\varepsilon}
&=\Big\{(w(\xi, \varepsilon), z(\xi, \varepsilon), \alpha(\xi, \varepsilon))
=\left((r,s)+\varepsilon {\bf{U}}(r, s, \alpha, \varepsilon), \alpha \right):
 \\
& \quad (r, s, \alpha)=\left(r(\xi, \varepsilon), s(\xi,
\varepsilon), \alpha(\xi, \varepsilon)\right), \xi\in(0,
C_\varepsilon) \Big\},
\end{aligned}
\end{equation}
where ${\bf{U}}(r, s, \alpha, \varepsilon)$ is defined in Lemma
\ref{lemma3.1}, $S(\xi, 0)=(\xi, f(\xi), g(\xi))$ and  $S(0,
\varepsilon)=(0, \beta, \alpha^*(\varepsilon))$. Here
$\alpha^*(\varepsilon)=\frac{\lambda^*(\varepsilon
\beta)}{\varepsilon}$, $C_{\varepsilon}$ is a certain smooth
positive function in $\varepsilon\in[0, \varepsilon_1]$ with $C_0=C$
and $\alpha(C_{\varepsilon}, \varepsilon)=A, w(C_\varepsilon,
\varepsilon), z(C_\varepsilon, \varepsilon)>0$ in $\Omega$.
\end{proposition}

\begin{proposition}\label{thm3.3}
Assume $\beta<0$,
$\|b\|_{\infty}\|d\|_{\infty}<\frac{\min_{\bar{\Omega}}\rho}{\|\rho\|_{\infty}}$.
Then for a sufficiently large number $A_1>0$, there also exist a
small $\varepsilon_2>0$ and a family of bounded curves 
$\{S(\xi, \varepsilon)=(\xi, \varepsilon)\in
[0, C_\varepsilon]\times[0, \varepsilon_2]\}$ of the form \eqref{71}
such that for any fixed $\varepsilon\in(0, \varepsilon_2]$, all
positive solutions of \eqref{37} with $\alpha \in
[-\frac{\beta}{\|d\|_{\infty}}, A_1 ]$ can be expressed
by $\Gamma_{\varepsilon}$ of the form \eqref{72}. Here $S(\xi,
\varepsilon)$  satisfies $S(\xi, 0)=(r_0+\xi, f(r_0+\xi),
g(r_0+\xi))$ and  $S(0, \varepsilon)=(\alpha_*(\varepsilon), 0,
\alpha_*(\varepsilon))$. Moreover,
$\alpha_*(\varepsilon)=\frac{\lambda_*(\varepsilon
\beta)}{\varepsilon}>0$, $C_\varepsilon$ is a smooth function in
$[0, \varepsilon_2]$ such that $C_0=C_1$ and $\alpha(C_\varepsilon,
\varepsilon)=A_1, w(C_\varepsilon, \varepsilon), z(C_\varepsilon,
\varepsilon)>0$ in $\Omega$.
\end{proposition}

An analysis of the limiting set $\{(r, f(r), g(r))\}$ deduces the
bifurcation structure of \eqref{37}.

\begin{theorem}\label{thm3.5}
Assume $\beta>0$,
$\|b\|_{\infty}\|d\|_{\infty}<\frac{\min_{\bar{\Omega}}\rho}{\|\rho\|_{\infty}}$,
$\fint_{\Omega}b(x)\rho(x)<\fint_{\Omega}b(x)\fint_{\Omega}\rho(x)$.
Then for any small constant $\eta>0$, there exists a small positive
number $\varepsilon_3$ such that if 
$(\beta, \varepsilon)\in [\frac{1-\fint_{\Omega}d(x)
\fint_{\Omega}b(x)}{\fint_{\Omega}b(x)
 \fint_{\Omega}\rho(x)-\fint_{\Omega}b(x)\rho(x)}+\eta, \eta^{-1} ]
 \times [0, \varepsilon_3]$,
the bifurcation direction at $(0, \beta, \alpha^*(\varepsilon))$ is
subcritical, and an unbounded $\subset$-shaped curve
$\Gamma^\varepsilon$ bifurcates from $(0, \beta,
\alpha^*(\varepsilon))$. While if 
$(\beta, \varepsilon)\in[\eta,
\frac{1-\fint_{\Omega}d(x)\fint_{\Omega}b(x)}{\fint_{\Omega}b(x)
 \fint_{\Omega}\rho(x)-\fint_{\Omega}b(x)\rho(x)}-\eta]\times [0, \varepsilon_3]$,
the bifurcation  at $(0, \beta, \alpha^*(\varepsilon))$ is
supercritical.
\end{theorem}

\begin{theorem}\label{thm3.6}
Assume $\beta<0$,
$\|b\|_{\infty}\|d\|_{\infty}<\frac{\min_{\bar{\Omega}}\rho}{\|\rho\|_{\infty}}$.
If $\min_{\bar{\Omega}}b(x)$ is very large and $\|d\|_{\infty}$ is
very small such that $g'(r_0)<0$, then for any small number
$\eta>0$, there exists $\varepsilon_4 >0$ such that if $(\beta,
\varepsilon)\in[-{\eta^{-1}}, -\eta]\times[0, \varepsilon_4]$, the
bifurcation at $(\alpha_*(\varepsilon), 0, \alpha_*(\varepsilon)) $
is subcritical, and  an unbounded $\subset$-shaped curve
$\Gamma_{\varepsilon}$ bifurcates from $(\alpha_*(\varepsilon), 0,
\alpha_*(\varepsilon))$; if $\|b\|_{\infty}$ is very small such that
$g'(r_0)>0$, then  the bifurcation at $(\alpha_*(\varepsilon), 0,
\alpha_*(\varepsilon))$ is supercritical for $(\beta,
\varepsilon)\in[-{\eta^{-1}}, -\eta]\times[0, \varepsilon_4]$.
\end{theorem}

The one-to-one correspondence  \eqref{32} between $(u,v)$ and
$(w,z)$ immediately yields the following result:

\begin{theorem} \label{thm3.7} 
If $\mu>0$ is sufficiently small, $k$ is sufficiently large,
and the assumptions in Theorem \ref{thm3.5} hold, then the set of
positive solutions of \eqref{02} forms an unbounded smooth curve
$$
\Gamma_p=\{\left(u(x;s), v(x;s), \lambda(s) \right): s>0\}
$$ 
with $\left(u(x;0), v(x;0), \lambda(0) \right)=(0, \mu,
\lambda^*)$ for a negative number $\lambda^*$. Furthermore, there
exists a small positive number $\mu^*$ such that the
following hold:
\begin{itemize}
\item[(i)] if $0<\mu\leq \mu^* /3$, then $\lambda'(0)>0$, $\Gamma_p$
supercritically bifurcates from $(0, \mu, \lambda^*)$;

\item[(ii)] if $2\mu^*/3\leq \mu \leq \mu^*$, then $\lambda'(0)<0$,
$\Gamma_p$ subcritically bifurcates from $(0, \mu, \lambda^*)$.
\end{itemize}
\end{theorem}

\begin{theorem}\label{thm3.8}
If $\mu<0$ is sufficiently close to $0$, $k$ is sufficiently large,
and $\|b\|_{\infty}\|d\|_{\infty}<\frac{\min_{\bar{\Omega}}\rho}{\|\rho\|_{\infty}}$,
then the set of positive solutions of \eqref{02} also  forms an
unbounded smooth curve
$$
\Gamma_p=\{\left(u(x;s), v(x;s), \lambda(s) \right): s>0 \},
$$
with $\left(u(x;0), v(x;0), \lambda(0) \right)=(\lambda_*, 0,
\lambda_*)$ for a positive number $\lambda_*$. Furthermore,  if
$\min b(x)$ is very large and $\|d(x)\|_{\infty}$ is very small, the
bifurcation direction is subcritical for $\mu_*\leq \mu <0$ with
some $\mu_*<0$; if $\|b\|_{\infty}$ is very small, the bifurcation
direction is supercritical for $\mu_*\leq \mu <0$.
\end{theorem}

\section{Main Results}

In this section, we give the stability and Hopf bifurcation results
of positive stationary solutions of \eqref{01}.

Firstly, we truncate $\Gamma_p$ shown in Theorems \ref{thm3.7} and
\ref{thm3.8} at every turning point with respect to the bifurcation
parameter $\lambda$. Denote all the local maximum or minimum points
of $\lambda(\xi)$ in $(0, C)$ by
\begin{equation*}
0<\xi_1<\xi_2<\dots<\xi_{n-1}<C.
\end{equation*}
Then if $\mu>0$, $(u(0), v(0))=(0, \mu)$, and $u(C), v(C)>0$; if
$\mu<0$, $(u(0), v(0))=(\lambda_*, 0)$ with $\lambda_*$ defined in
Theorem \ref{thm3.8}, and $u(C), v(C)>0$. It should be noted that
$\lambda(\xi)$ possesses at least one local minimum point if
$\Gamma_p$ is $\subset$-shaped.  Moreover, we set
$$
\Gamma_p(j)=\{(u(\xi), v(\xi), \lambda(\xi))\in \Gamma_p:
 \xi\in (\xi_{j-1}, \xi_j)\}
 $$
for each $1\leq j\leq n$ with $\xi_0=0$ and $\xi_n=C$. Therefore,
$$
\cup_{j=1}^{n}\Gamma_p(j)=\Gamma_p\setminus
\cup_{j=1}^{n-1}\{(u(\xi_j), v(\xi_j), \lambda(\xi_j))\}.
$$ 
As will be shown in Section 4, one can see that, different from the
predator-prey system, the number $n-1$ of the turning points of
$\lambda(\xi)$ can be determined. More precisely, if $\Gamma_p$ is
$\subset$-shaped, then $n=2\ell$ for a positive integer
$\ell$; if the bifurcation direction is supercritical,
then $n=2\ell-1$ for some positive integer $\ell$.

 Now we show the main results obtained in the paper.
 
\begin{theorem}\label{thm2.1}
Let $\mu=\varepsilon \beta>0$, $k=1/\varepsilon$. If the assumptions
in Theorem \ref{thm3.5} hold, then for almost every $\mu>0$, there
exist three positive small numbers $\delta, \mu^*$ and
$\varepsilon_0$ such that when
$$
2\mu^*/3 \leq \mu\leq \mu^*, \quad d_1/d_2\leq\delta, \quad
\varepsilon\leq \varepsilon_0,
$$ 
then $n=2\ell$, and all positive solutions on 
$\Gamma_p(2j) (j=1,2,\dots, \ell)$ are asymptotically stable in 
the topology of $X$, while all positive solutions on 
$\Gamma_p(2j-1)(j=1,2,\dots, \ell)$ are unstable; when
$$
0<\mu\leq\mu^*/3,\quad d_1/d_2\leq\delta, \quad
\varepsilon\leq \varepsilon_0,
$$
then $n=2\ell-1$, and all positive solutions on
 $\Gamma_p(2j-1) (j=1,2,\dots, \ell)$ are
asymptotically stable in the topology of $X$, while all  positive
solutions on $\Gamma_p(2j)(j=1,2,\dots, \ell-1)$ are unstable.
\end{theorem}

\begin{theorem}\label{thm2.2}
Let $\mu=\varepsilon \beta<0$, $k=1/\varepsilon$, and
$\|b\|_{\infty}\|d\|_{\infty}<\min_{\bar{\Omega}}\rho/\|\rho\|_{\infty}$.
Then if $\min_{\bar{\Omega}}b(x)$ is very large and $\|d\|_{\infty}$
is very small,  for almost every $\mu<0$, there exist three positive
small numbers $\delta, -\mu_*$ and $\varepsilon_0$ such that when
$$
\mu_* \leq \mu<0, \quad d_1/d_2\leq\delta, \quad
\varepsilon\leq \varepsilon_0,
$$ 
the first stability
conclusion in Theorem \ref{thm2.1} holds; if $\|b\|_{\infty}$ is
very small, then under the same conditions, the second stability
conclusion in Theorem \ref{thm2.1} holds.
\end{theorem}

From Theorems \ref{thm2.1} and \ref{thm2.2}, we see that when the
spatial heterogeneity produces multiple positive stationary
solutions in the subcritical case, if $u$ moves much slower than
$v$, then at least one of the multiple positive stationary solutions
is unstable and the other one is stable. In
particular, unstable positive stationary solutions bifurcate from
semitrivial solutions, which implies that the spatial heterogeneity
cannot have a strongly beneficial effect on the species in low
densities.

Next we assume that the segregation condition of $b(x)$
and $\rho(x)$
\begin{equation}\label{22}
\fint_{\Omega}\frac{b(x)}{1+r\rho(x)}\fint_{\Omega}
\frac{\rho(x)}{(1+r\rho(x))^2}>\fint_{\Omega}\frac{b(x)\rho(x)}{(1+r\rho(x))^2}
\fint_{\Omega}\frac{1}{1+r\rho(x)}
\end{equation}
holds for  $r\in [r_0, C_0+r_0]$ in case $\beta<0$. In fact, we can
show that \eqref{22} does hold under a spatial segregation of $b(x)$
and $\rho(x)$. Precisely, for any small $\varepsilon$ satisfying
$\varepsilon<\frac{\fint_{\Omega}b(x)}{1+(C_0+r_0)\|\rho\|_{\infty}}$,
if ${\rm{supp}} \,\rho\cap {\rm{supp}} (b-\varepsilon)_+=\emptyset$,
then
\begin{align*}
\fint_{\Omega}\frac{1}{1+r\rho(x)}\fint_{\Omega}\frac{b(x)\rho(x)}
{(1+r\rho(x))^2}
&\leq\varepsilon\fint_{\Omega}\frac{1}{1+r\rho(x)}
\fint_{\Omega}\frac{\rho(x)}{(1+r\rho(x))^2}\\
&\leq\varepsilon\fint_{\Omega}\frac{\rho(x)}{(1+r\rho(x))^2}\\
&<\fint_{\Omega}\frac{b(x)}
{1+(C_0+r_0)\|\rho\|_{\infty}}\fint_{\Omega}\frac{\rho(x)}{(1+r\rho(x))^2}\\
&\leq\fint_{\Omega}\frac{b(x)}{1+r\rho(x)}\fint_{\Omega}
\frac{\rho(x)}{(1+r\rho(x))^2}.
\end{align*}

\begin{remark} \label{rmk3.3} \rm 
We  point out that the segregation condition  \eqref{22}
is equivalent to
\begin{equation}
\label{30}
\int_{\Omega}\int_{\Omega}\frac{(b(x)-b(y))(\rho(x)-\rho(y))}{(1+ r
\rho(x))^2(1+ r \rho(y))^2}<0.
\end{equation} From the equivalent
inequality \eqref{30}, we see that if $\rho(x)=f(b(x))$ for some
strictly decreasing function $f$ and $b(x)\not\equiv$constant, then
\eqref{30} holds, i.e., \eqref{22} holds. In particular, when the
spatial dimension is $1$ and $\Omega$ is an interval, if $b(x)$ is
strictly increasing and $\rho(x)$ is strictly decreasing, then
\eqref{22} and \eqref{30} also hold.

Therefore, the segregation between $b(x)$ and $\rho(x)$ does hold
under certain circumstances. 
\end{remark}


One will see that if $d_1/d_2$ becomes sufficiently large, the
segregation of $\rho(x)$ and $b(x)$ can cause Hopf bifurcation on
the positive stationary solutions of $\Gamma_p$ in case $\mu<0$.

\begin{theorem}\label{thm2.4}
Let $\mu=\varepsilon \beta<0$, $k=1/\varepsilon$, and
$\|b\|_{\infty}\|d\|_{\infty}<\min_{\bar{\Omega}}\rho/\|\rho\|_{\infty}$.
Suppose $b(x)$ and $\rho(x)$ satisfy the segregation condition
\eqref{22}. Then if $-\beta$ is sufficiently large, and
$\|b\|_{\infty}$ is small,  there exist a large number $D>0$ and a
small number $\varepsilon_0>0$ such that if $\frac{d_1}{d_2}\geq D$
and $\varepsilon\leq \varepsilon_0$, Hopf bifurcation appears at a
certain point on $\Gamma_p$.
\end{theorem}

Note that in Theorem \ref{thm2.4}, small $\|b\|_{\infty}$ deduces
$g'(r_0)>0$. Thus, the bifurcation curve is not fish-hook shaped.

 By the stability result in Section 4 and the Hopf bifurcation
 result in Section 5,
 we can see much clearer that: when $d_1/d_2$ is small enough, the stability
 is rather clear, and no Hopf bifurcation occurs due to \eqref{48}; while as $d_1/d_2$
 becomes large, some stable positive stationary
solutions bifurcating from $(\lambda_*, 0)$ for $\mu<0$ will lose
their stability, and Hopf bifurcation occurs.

\section{Stability Analysis}

 In the section, we will deduce the stability result of positive
 stationary solutions of \eqref{33}. Since the change of variables in
 \eqref{32} is regular, the stability of positive stationary
solutions $(w,z)=(u/\varepsilon, (1+k\rho(x)u)v/\varepsilon)$ of
\eqref{33} immediately yields that of the positive stationary
solutions $(u, v)$ of \eqref{01}. Therefore, we only need  to study
the stability of positive stationary solutions on
$\Gamma^\varepsilon$ and $\Gamma_\varepsilon$ given in
 Propositions \ref{thm3.2} and \ref{thm3.3}.

 \subsection{Linearized Stability}

 We firstly deduce the linearized stability. Note that the positive
 stationary solutions of \eqref{33} with $\alpha \in [-c\beta \|b\|_{\infty},
 A]$ in case $\beta>0$
 and $\alpha\in [-\beta / \| d\| _{\infty}, A_1] $ in case $\beta<0$ can be
  parameterized as
$$
\Gamma^\varepsilon(\Gamma_\varepsilon)=
\{(w(\xi, \varepsilon), z(\xi, \varepsilon), \alpha(\xi,
\varepsilon)): \xi\in (0, C_\varepsilon)\}
$$ 
for small  $\varepsilon>0$. Then for any
 $(w(\xi, \varepsilon), z(\xi, \varepsilon),
 \alpha(\xi, \varepsilon))\in \Gamma^\varepsilon(\Gamma_\varepsilon)$,
 we define the linearized operator $L(\xi, \varepsilon): X\to
 Y$ by
 \begin{equation*}
 L(\xi, \varepsilon)\binom{h}{k}=H\binom{h}{k}+\varepsilon
 B_{(w,z)}\left(w(\xi, \varepsilon), z(\xi, \varepsilon), \alpha(\xi,
 \varepsilon)\right)\binom{h}{k},
 \end{equation*}
where $B_{(w,z)}$ denotes the Fr\'{e}chet derivative of $B$ with
respect to $(w,z)$. By virtue of the left-hand side of \eqref{33},
we further set
\begin{equation*}
J(\xi, \varepsilon)=\begin{pmatrix} \frac{1}{d_1} & 0\\
-\frac{\rho(x)z(\xi,
\varepsilon)}{d_2(1+\rho(x)w(\xi,\varepsilon))^2}
&\frac{1}{d_2(1+\rho(x)w(\xi, \varepsilon))}
\end{pmatrix}.
\end{equation*}
Substituting
$$
(w,z)=\left(w(\xi, \varepsilon)+h e^{-\lambda t},
z(\xi, \varepsilon)+k e^{-\lambda t}\right)
$$ 
into \eqref{33} and
neglecting the higher order terms, one sees that the linearized
eigenvalue problem associated with $(w(\xi, \varepsilon), z(\xi,
\varepsilon))$ is given by
\begin{equation}\label{42}
 L(\xi, \varepsilon)\binom{h}{k}=-\lambda J(\xi,
 \varepsilon)\binom{h}{k}.
 \end{equation}


In the following, we  use  the spectral theory to show the
linearized stability of positive stationary solutions on
$\Gamma^\varepsilon (\Gamma_\varepsilon)$.

\begin{lemma}\label{lemma4.1}
Let $\{\lambda_j(\xi, \varepsilon)\} \left(\operatorname{Re}\lambda_j(\xi,
\varepsilon)\leq \operatorname{Re}\lambda_{j+1}(\xi, \varepsilon)\right)$
be the eigenvalues (counting multiplicity) of \eqref{42}. If
$\varepsilon>0$ is sufficiently small, then the following holds:
\begin{equation*}
\lim_{\varepsilon\to 0}\lambda_1(\xi,
\varepsilon)=\lim_{\varepsilon\to 0}\lambda_2(\xi,
\varepsilon)=0
\end{equation*}
and ${\rm{Re}}\lambda_j(\xi, \varepsilon)>\kappa$ for $j\geq3$ and
$\xi\in (0, C_\varepsilon)$
 with some positive constant $\kappa$ independent of $(\xi, \varepsilon)$.
\end{lemma}

\begin{proof}
We  give only the proof of the case $\beta>0$, since the
proof of the case $\beta<0$ is similar.
Proposition \ref{thm3.2} asserts that
$$
(w(\xi, \varepsilon), z(\xi, \varepsilon), \alpha(\xi, \varepsilon))
\to (\xi, f(\xi),
g(\xi))\quad\text{in }C^1(\bar{\Omega})\times C^1(\bar{\Omega})\times
\mathbb{R}
$$ 
as $\varepsilon\to 0$ for any $\xi\in (0,C_\varepsilon)$. 
Then as $\varepsilon\to 0$, \eqref{42} reduces to
\begin{equation}
\begin{gathered}
 -d_1\Delta h=\lambda h,\quad x\in \Omega,\\
 -d_2\Delta k=\lambda\left(\frac{1}{1+\xi \rho(x)}k-
 \frac{\rho(x)f(\xi)}{(1+\xi\rho(x))^2}h\right), \quad  x\in \Omega, \\
 \partial _{\nu}h=\partial _{\nu} k=0, \quad x\in \partial \Omega.
 \end{gathered} \label{81}
 \end{equation}
 The eigenvalues of \eqref{81} comprise only $\{\bar{\lambda}_{j}\} \cup
 \{\tilde{\lambda}_{j}\}$, where $\bar{\lambda}_{j}$ and
 $\tilde{\lambda}_{j}$ are eigenvalues of
 \begin{equation}
\begin{gathered}
 -d_1\Delta h=\lambda h,\quad x\in \Omega,\\
 \partial _{\nu}h=0, \quad x\in \partial \Omega,
 \end{gathered}
 \label{82}
 \end{equation} and
\begin{equation}
\begin{gathered}
 -d_2\Delta k=\lambda\frac{1}{1+\xi \rho(x)}k, \quad
 x\in \Omega, \\
 \partial _{\nu} k=0, \quad x\in \partial \Omega,
 \end{gathered} \label{83}
 \end{equation}
respectively. Since both of the principal  eigenvalues of \eqref{82}
 and \eqref{83} are zero, and all the other eigenvalues possess
 positive real parts and are bounded away from zero. Thus the
 limiting problem \eqref{81} has a double eigenvalue $\lambda=0$,
 and the other eigenvalues have positive real parts. Then the perturbation theory
by Kato \cite[Chapter 8]{kato} yields the  lemma.
\end{proof}

As $\{\lambda_j(\xi, \varepsilon)\}$ is a symmetric set with respect
to the real axis in $\mathbb{C}$, the eigenvalues $\lambda_1(\xi,
\varepsilon)$ and $\lambda_2(\xi, \varepsilon)$ (shown in Lemma
\ref{lemma4.1}) must satisfy either (i) or (ii):

(i) both of $\lambda_1(\xi, \varepsilon)$ and $\lambda_2(\xi,
\varepsilon)$ are real numbers;

(ii) $\lambda_1(\xi, \varepsilon)$ is a complex conjugate of
$\lambda_2(\xi, \varepsilon)$.

In the sequel, we always assume that $ \operatorname{Re}\lambda_1(\xi,
\varepsilon)\leq \operatorname{Re}\lambda_2(\xi, \varepsilon)$ and
$\operatorname{Im}\lambda_1(\xi, \varepsilon) \geq
\operatorname{Im}\lambda_2(\xi, \varepsilon)$.

The definition of the linearized stability of positive stationary
solutions on $\Gamma^\varepsilon (\Gamma_\varepsilon)$ can be given
as follows.

\begin{definition}\label{def4.2} \rm
If $\operatorname{Re}\lambda_1(\xi, \varepsilon)>0$, then  
$(w(\xi, \varepsilon), z(\xi, \varepsilon))$ of \eqref{33} 
is called linearly stable; if $\operatorname{Re}\lambda_1(\xi, \varepsilon)<0$, 
it is called linearly unstable.
\end{definition}

From the definition, we see that the linearized stability of any
positive stationary solution $(w(\xi, \varepsilon), z(\xi,
\varepsilon))$ on $\Gamma^\varepsilon (\Gamma_\varepsilon)$ is
determined by the sign of $\operatorname{Re}\lambda_1(\xi, \varepsilon)$.
A similar argument to that of Lemma 5.3 in \cite{kuto} or Lemma 4.3
in \cite{kuto1} can further deduce the following lemma associated
with $\lambda_1(\xi, \varepsilon)$ and 
$\lambda_2(\xi,\varepsilon)$.

\begin{lemma}\label{lemma4.3}
Let $\lambda_1(\xi, \varepsilon)$ and $\lambda_2(\xi, \varepsilon)$
be eigenvalues of \eqref{42} shown in Lemma \ref{lemma4.1}. Then for
any fixed $r\in (0, C_0)$, we  have
\begin{equation*}
\lim_{(\xi, \varepsilon)\to (r,0)}\frac{\lambda_j(\xi,
\varepsilon)}{\varepsilon}=\mu_j(r) \quad (j=1,2)
\end{equation*}
in the case $\beta>0$; and
\begin{equation*}
\lim_{(\xi, \varepsilon)\to (r,0)}\frac{\lambda_j(\xi,
\varepsilon)}{\varepsilon}=\mu_j(r+r_0) \quad (j=1,2)
\end{equation*}
in the case $\beta<0$, where $\mu_j(r)$ satisfying
$\operatorname{Re}\mu_1(r)\leq \operatorname{Re}\mu_2(r)$ and $\operatorname{Im}
\mu_1(r) \geq \operatorname{Im}\mu_2(r)$ are eigenvalues of
\begin{equation}\label{460}
M(r)=-J(r)^{-1}\Phi^0_{(r,s)}(r, f(r), g(r)),
\end{equation}
where $\Phi^0_{(r,s)}(r, f(r), g(r))$ denotes the Jacobian matrix of
$\Phi^0$, and
\begin{equation*}
J(r)={\begin{pmatrix} \frac{1}{d_1} & 0\\
-\frac{f(r)}{d_2}\fint_{\Omega}\frac{\rho(x)}{(1+r\rho(x))^2}
&\fint_{\Omega}\frac{1}{d_2(1+r\rho(x))}
\end{pmatrix}}.
\end{equation*}
\end{lemma}


By some calculations, we can show that
\begin{align*}
&\Phi^0_{(r,s)}(r, f(r), g(r))\\
&={\begin{pmatrix} -r[1+f(r)
\fint_\Omega \frac{b(x)\rho(x)}{(1+r\rho(x))^2} ]& r\fint_\Omega \frac{b(x)}{1+r\rho(x)}\\
f(r)[\fint_\Omega\frac{d(x)-\beta
\rho(x)}{(1+r\rho(x))^2}+2f(r)\fint_{\Omega}\frac{\rho(x)}{(1+r\rho(x))^3}]
&-f(r)\fint_{\Omega}\frac{1}{(1+r\rho(x))^2}
\end{pmatrix}}.
\end{align*}
It can also be verified that
\begin{equation*}
\Phi^0_{(r,s)}(r, f(r), g(r))={\begin{pmatrix} -r[g'(r)+f'(r)
\fint_\Omega \frac{b(x)}{1+r\rho(x)} ]& r\fint_\Omega \frac{b(x)}{1+r\rho(x)}\\
f(r)f'(r)\fint_\Omega\frac{1}{(1+r\rho(x))^2}
&-f(r)\fint_{\Omega}\frac{1}{(1+r\rho(x))^2}
\end{pmatrix}},
\end{equation*}
from which we know that
\begin{equation}\label{390}
\det  \Phi^0_{(r, s)}(r, f(r), g(r))=rf(r)g'(r)\fint_\Omega
\frac{1}{(1+r\rho(x))^2}.
\end{equation}

By the perturbation theory of the Fredholm operator
 developed by Du and Lou \cite{du2}, we can further deduce the following lemma
characterizing the degenerate solution
 ($\lambda_1(\xi, \varepsilon)=0$ or
 $\lambda_2(\xi, \varepsilon)=0$ for some $\xi\in (0,
 C_\varepsilon)$).
 
 \begin{lemma}\label{lemma4.4}
 Assume that $\varepsilon>0$ is small enough. Then
  $(w(\xi^*,\varepsilon), z(\xi^*, \varepsilon), \alpha(\xi^*,
  \varepsilon))$ for some $\xi^* \in (0, C_\varepsilon)$ is a
  degenerate solution if and only if
  $$\partial_\xi \alpha(\xi^*, \varepsilon)=0.$$
\end{lemma}

Next we show that $\lim_{r\to +\infty}g'(r)>0$. Due to
\eqref{310}, some calculations yield that
$$
g'(r)=1-f'(r)\fint_\Omega \frac{b(x)}{1+r\rho
(x)}+f(r)\fint_\Omega \frac{b(x)\rho(x)}{(1+r\rho(x))^2}
$$
and
$$
\lim_{r\to +\infty}
g'(r)=1-\fint_\Omega\frac{b(x)}{\rho(x)} 
\fint_\Omega\frac{d(x)}{\rho(x)} \Big(\fint_\Omega \frac {1}{\rho^2(x)}\Big)^{-1}.
$$ 
Thus under the weak cooperation
condition, $\lim_{r\to +\infty}g'(r)>0$ holds true. Then for
large number $C_0$ shown in Propositions \ref{thm3.2} and
\ref{thm3.3}, we have that
\begin{equation*}
g'(C_0)>0\quad{\rm{and}}\quad g'(C_0+r_0)>0.
\end{equation*}

 Since $g$ is analytic, and $g'(r)>0$ for all large $r$, $g'(r)=0$
 must possess at most  finitely many solutions $r_i$. 
 Then the finiteness
deduces that any zero of $g'$ must be a strictly critical point of
$g$ for almost every $\beta$. For such $\beta$, we denote all the
zeros of $\partial_\xi \alpha(\xi, \varepsilon)$ by
$$
0<\xi_1(\varepsilon)<\xi_2(\varepsilon)<\dots 
<\xi_{n-1}(\varepsilon)<C_\varepsilon
$$
when $\varepsilon>0$ is sufficiently small. So,
$$
\left(w_i, z_i, \alpha^i\right)=\left(w(\xi_i(\varepsilon), \varepsilon),
z(\xi_i(\varepsilon), \varepsilon), \alpha(\xi_i(\varepsilon),
\varepsilon)\right) \quad\text{for }1\leq i\leq n-1
$$ 
are all turning
points on $\Gamma^\varepsilon(\Gamma_\varepsilon)$ with respect to
the bifurcation parameter $\alpha$ in either case $\beta>0$ or case
$\beta<0$. Then we truncate $\Gamma^\varepsilon(\Gamma_\varepsilon)$
at every turning point as
$$
\Gamma^\varepsilon(i)(\Gamma_\varepsilon(i))=\{(w(\xi, \varepsilon), z(\xi, \varepsilon),
\alpha(\xi, \varepsilon)): \xi\in (\xi_{i-1}(\varepsilon),
\xi_{i}(\varepsilon))\}
$$ 
for $1\leq i\leq n$, with
$\xi_0(\varepsilon)=0$ and $\xi_n(\varepsilon)=C_\varepsilon$.
Therefore,
$$
\cup_{i=1}^{n}\Gamma^\varepsilon(i)
(\Gamma_\varepsilon(i))=\Gamma^\varepsilon(
\Gamma_\varepsilon)\setminus\cup_{i=1}^{n-1} \left\{\left(w_i,
z_i, \alpha^i\right)\right\}.
 $$


\begin{lemma}\label{lemma4.5}
For almost every $\beta>0$, under the assumptions of Theorem
\ref{thm3.5}, there exist two small positive constants $\delta$ and
$\varepsilon_0$ such that if $d_1/d_2 \leq \delta$, $\varepsilon\leq
\varepsilon_0$ and the bifurcation at $(0, \beta, \alpha^*)$ is
subcritical, then $n=2\ell$ for some positive integer $\ell$, and
all positive stationary solutions are linearly unstable on
$\Gamma^\varepsilon(2j-1) (j=1,2,\dots, \ell)$, and linearly stable
on $\Gamma^\varepsilon(2j) (j=1,2,\dots, \ell)$; if the bifurcation
direction is supercritical, then $n=2\ell-1$, and all positive
stationary solutions are linearly stable on
$\Gamma^\varepsilon(2j-1) (j=1,2,\dots, \ell)$, and linearly
unstable on $\Gamma^\varepsilon(2j) (j=1,2,\dots, \ell-1)$.
\end{lemma}

\begin{proof}
From the expression of $M(r)$, we can obtain that
\begin{align*}
&(\mu_1(r)+\mu_2(r))\fint_\Omega\frac{1}{1+r\rho(x)}\\
&=d_2\left\{f(r)\fint_\Omega\frac{1}{(1+r\rho(x))^2} +\frac{r
d_1}{d_2}[\fint_\Omega\frac{1}{1+r\rho(x)}-f(r)K(r)]\right\},
\end{align*}
where
$$
K(r)=\fint_\Omega\frac{b(x)}{1+r\rho(x)}
\fint_\Omega\frac{\rho(x)}{(1+r\rho(x))^2}-
\fint_\Omega\frac{b(x)\rho(x)}{(1+r\rho(x))^2}
\fint_\Omega\frac{1}{1+r\rho(x)}.
$$
Then if $\frac{d_1}{d_2}$ is sufficiently small, we have
$$
\mu_1(r)+\mu_2(r)>0 \quad\text{for }r\in[0, C_0].
$$
So Lemma \ref{lemma4.3} yields that if $\varepsilon>0$ is
sufficiently small,
\begin{equation}\label{48}
\lambda_1(\xi, \varepsilon)+\lambda_2(\xi,
\varepsilon)>0 \quad\text{for }\xi\in[0, C_\varepsilon].
\end{equation}
Furthermore, we can show that
\begin{equation*}
\mu_1(r)\mu_2(r)=d_1d_2
rf(r)g'(r)\fint_\Omega\frac{1}{(1+r\rho(x))^2}\Big(\fint_\Omega
\frac{1}{1+r\rho(x)}\Big)^{-1},
\end{equation*}
which means that
\begin{equation}\label{410}
\operatorname{sign}\mu_1(r)\mu_2(r)=\operatorname{sign}g'(r)
~\quad\text{for }~r\in(0, C_0).
\end{equation}
Therefore, for any fixed $r\in(0, C_0)$, if $g'(r)>0$ and $(\xi,
\varepsilon)$ is near $(r, 0)$, then $\lambda_1(\xi,
\varepsilon)\lambda_2(\xi, \varepsilon)>0$. Together with
\eqref{48}, we deduce that $\operatorname{Re} \lambda_1(\xi,
\varepsilon)>0$; while if $g'(r)<0$ and $(\xi, \varepsilon)$ is near
$(r, 0)$, then $\lambda_1(\xi, \varepsilon)\lambda_2(\xi,
\varepsilon)<0$, and $\operatorname{Re} \lambda_1(\xi, \varepsilon)<0$.
Moreover, if $\varepsilon>0$ is sufficiently small, $\operatorname{Re}
\lambda_2(\xi, \varepsilon)>0$ holds for all $\xi\in [0,
C_\varepsilon]$ by \eqref{48}, then $\lambda_1(\xi, \varepsilon)=0$
if and only if $\xi=\xi_i(\varepsilon)$ for some $1\leq i\leq n-1$.

Additionally, under the assumptions of Theorem \ref{thm3.5}, we know
that if the bifurcation direction is subcritical, then $g'(0)<0$ and
$g'(C_0)>0$. Then the number $n-1$ of turning points of
$\alpha(\xi)$ must be odd. If the bifurcation direction is
supercritical, then $g'(0)>0$, $g'(C_0)>0$, and $n-1$ is even. Thus
the conclusions in the lemma are proved.
\end{proof}

In the case $\beta<0$, since
$$\mu_1(r_0)+\mu_2(r_0)=r_0 d_1>0,$$
we see that $\mu_1(r)+\mu_2(r)>0$ for $r\in [r_0, r_0+\delta]$ with
a small positive number $\delta$. By virtue of $f(r)>0$ for
$r\in[r_0+\delta, C_0+r_0]$, we can further choose $d_1/d_2$
sufficiently small such that
$$
\mu_1(r)+\mu_2(r)>0 \quad\text{for }r\in[r_0+\delta, C_0+r_0].
$$
Combining the above, we know
$$
\mu_1(r)+\mu_2(r)>0\quad\text{for }r\in[r_0, C_0+r_0].
$$
 A similar argument to the proof of Lemma
\ref{lemma4.5} deduces the following lemma.

 \begin{lemma}\label{lemma4.7}
For almost every $\beta<0$, under the assumptions of Theorem
 \ref{thm3.6}, there exist two small positive constants $\delta$ and
$\varepsilon_0$ such that if $d_1/d_2 \leq \delta$, $\varepsilon\leq
\varepsilon_0$ and the bifurcation at $(\alpha_*, 0, \alpha_*)$ is
subcritical, then the same conclusions as those of the subcritical
case shown in Lemma \ref{lemma4.5} hold; if the bifurcation
direction is supercritical, then the same conclusions as those of
the supercritical case shown in Lemma \ref{lemma4.5} hold
\end{lemma}

From Lemmas \ref{lemma4.5} and \ref{lemma4.7}, together with 
\cite[Lemma 4.5]{kuto1} and \cite[Lemma 5.5]{kuto}, we can see that
under large cross-diffusion effect for one species and comparatively
small natural diffusion effect for the other species, the stability
of positive stationary solutions changes at every turning point of
the bifurcation curve with respect to the bifurcation parameter in
either Neumann or Dirichlet boundary condition.

\begin{remark} \label{rmk4.7} {\rm
As pointed out in the previous paper, if all coefficients are
spatially homogeneous; i.e., $\rho(x)\equiv$ const., $b(x)\equiv $
const. and $d(x)\equiv$ const., then
$$
f(r)=(\beta+rd)(1+r\rho),\quad g(r)=r-b(\beta+rd).
$$
Under the weak cooperation condition $bd<1$, we have $g'(r)=1-bd>0$.
Thus when $\varepsilon>0$ is small enough,
$$
\alpha_{\xi}(\xi,\varepsilon)>0.
$$
Then \eqref{37} has a unique positive solution if $\alpha\in
(\alpha^*(\varepsilon), \infty)$ and no positive solutions if
$\alpha\leq \alpha^*(\varepsilon)$ in case $\beta>0$. If $\beta<0$,
$\alpha^*(\varepsilon)$ should be replaced by
$\alpha_*(\varepsilon)$.

Next, we look at the linearized stability of the unique positive
solution on the bifurcation curve.  At this time,
$$
\mu_1(r)+\mu_2(r)=d_2\Big(\beta+rd+r\frac{d_1}{d_2}\Big).
$$
Then if $\beta>0$, $\mu_1(r)+\mu_2(r)>0$ always holds for 
$r\in [0, C_0]$ regardless of the values  of $d_1, d_2, r$ and $d$; if
$\beta<0$, since $r\geq r_0$, $\mu_1(r)+\mu_2(r)>0$
 also holds for $r\in[r_0, C_0+r_0]$. Furthermore,
$$
\operatorname{sign}\mu_1(r)\mu_2(r)=\operatorname{sign}g'(r)>0.
$$
So we see that if the environment is homogeneous, all the unique
positive stationary solutions are linearly stable, non-degenerate
and Hopf bifurcation can never occur on
$\Gamma^\varepsilon(\Gamma_\varepsilon)$.

Whereas, when the environment is heterogeneous and the heterogeneity
causes multiple positive stationary solutions, if the natural
diffusion rate $d_1$ of the first cooperator is very small
comparatively to that of the second cooperator, then at least one of
the multiple coexistence states is unstable. Furthermore, Hopf
bifurcation can be shown to occur under suitable conditions in
Section 5, which is quite different from that of the homogeneous
environment.}
\end{remark}


\subsection{Asymptotic stability}


 By the linearization  principle for quasilinear parabolic
equations developed by Potier-Ferry \cite{ferry}, and the
interpolation spaces $[X, Y]_{\theta, p}$ $(0\leq \theta\leq 1)$ in
the sense of Lions-Peetre \cite{lions}, we can show that the
linearized stability implies the asymptotic stability. One can refer
to \cite{kuto1} and \cite{kuto} for the details. More precisely, we
have the following lemma:

\begin{lemma}\label{lemma4.6}
Under the assumptions of Lemmas
\ref{lemma4.5} and \ref{lemma4.7}, all linearly stable positive
stationary solutions on $\Gamma^\varepsilon$ or $\Gamma_\varepsilon$
are asymptotically stable in the topology of $X$, and all linearly
unstable positive stationary solutions on $\Gamma^\varepsilon$ or
$\Gamma_\varepsilon$ are unstable.
\end{lemma}

The regularity of the scaling \eqref{32} immediately yields Theorems
\ref{thm2.1} and \ref{thm2.2}.

\section{Hopf Bifurcation}


In this section, we will give the Hopf bifurcation of positive
stationary solutions of \eqref{33}. To do so,  set
\begin{equation*}
\beta=m \tilde{\beta} ,\quad d(x)=m\tilde{d}(x)
\end{equation*}
for $\tilde{\beta}\in \mathbb{R}$ and nonnegative function
$\tilde{d}(x)$. Then $f(r)$ can be expressed as
\begin{equation*}
f(r)=m\fint_\Omega \frac{\tilde{\beta}+r\tilde{d}(x)}{1+r
\rho(x)}\Big(\fint_\Omega\frac{1}{(1+r \rho(x))^2}\Big)^{-1}.
\end{equation*}

In the ncase $\beta>0$, we failed to obtain Hopf bifurcation on the
bifurcation continuum. To the best of our knowledge, we can only
give Hopf bifurcation when $\beta<0$ and the bifurcation direction
at $(\alpha_*, 0)$ is supercritical.


\begin{proposition}\label{proposition5.1}
Assume $\beta<0$,
$\|b\|_{\infty}\|d\|_{\infty}<\frac{\min_{\bar{\Omega}}\rho}{\|\rho\|_{\infty}}$,
$\|b\|_{\infty}$ is very small such that the bifurcation at $(
\alpha_*, 0)$ is supercritical, then if $\rho(x)$ and $b(x)$ satisfy
the segregation condition \eqref{22}, and $m>0$ is sufficiently
large,  there exist a large number $D>0$ and a small number
$\varepsilon_0>0$ such that if $d_1/d_2\geq D$ and $\varepsilon\leq
\varepsilon_0$, Hopf bifurcation occurs at a certain point on
$\Gamma^\varepsilon$.
\end{proposition}

\begin{proof}
To prove the proposition, we take two steps: at the first step, we
show that under the conditions of the proposition, for the
eigenvalues $\mu_1(r)$ and $\mu_2(r)$ of $M(r)$ defined by
\eqref{460}, there exists $\bar{r}>r_0$ such that
$\mu_1(\bar{r})+\mu_2(\bar{r})=0, \mu_1(\bar{r})\mu_2(\bar{r})>0$
and $\mu_1'(\bar{r})+\mu_2'(\bar{r})<0$.

Note that
$$
K(r)=\fint_\Omega\frac{b(x)}{1+r\rho(x)}
\fint_\Omega\frac{\rho(x)}{(1+r\rho(x))^2}-
\fint_\Omega\frac{b(x)\rho(x)}{(1+r\rho(x))^2}
\fint_\Omega\frac{1}{1+r\rho(x)}>0
$$
for $r\in[r_0, C_0+r_0]$ is assumed. Due to the expression of $f(r)$,
\begin{align*}
&f(r)K(r)-\fint_\Omega\frac{1}{1+r\rho(x)}\\
&=m\fint_\Omega \frac{\tilde{\beta}+r\tilde{d}(x)}{1+r
\rho(x)}\left(\fint_\Omega\frac{1}{(1+r
\rho(x))^2}\right)^{-1}K(r)-\fint_\Omega\frac{1}{1+r\rho(x)}.
\end{align*}
There exists a large number $M_1>0$ such that if $m\geq M_1$,
$$
f(r)K(r)-\fint_\Omega\frac{1}{1+r\rho(x)}>0 \quad\text{for }
r\in[r_0, C_0+r_0].
$$
 As
\begin{align*}
\mu_1(r)+\mu_2(r)
&= d_2\Big\{f(r)\fint_\Omega\frac{1}{(1+r\rho(x))^2}
\Big(\fint_\Omega\frac{1}{1+r\rho(x)}\Big)^{-1} \\
&\quad -\frac{rd_1}{d_2}[f(r)K(r)
\Big(\fint_\Omega\frac{1}{1+r\rho(x)}\Big)^{-1}-1]\Big\},
\end{align*}
then
\begin{equation*}
\mu_1(r_0)+\mu_2(r_0)=r_0d_1>0.
\end{equation*} 
Furthermore, \eqref{410} implies that
$\mu_1(r_0)\mu_2(r_0)>0$. Since
\begin{equation*}
\begin{split}
\mu_1'(r_0)+\mu_2'(r_0)
&=d_2\Big[f'(r_0)\fint_\Omega\frac{1}{(1+r_0\rho(x))^2}
\Big(\fint_\Omega\frac{1}{1+r_0\rho(x)}\Big)^{-1}\\
&\quad -\frac{d_1}{d_2}\Big(r_0f'(r_0)K(r_0)
\Big(\fint_\Omega\frac{1}{1+r_0\rho(x)}\Big)^{-1}-1\Big)\Big],
\end{split}
\end{equation*}
$$
f'(r_0)=m\fint_\Omega \frac{\tilde{d}(x)-\tilde{\beta} \rho(x)}
{(1+r_0\rho(x))^2}\Big(\fint_\Omega\frac{1}
{(1+r_0\rho(x))^2}\Big)^{-1}>0,$$ there exists a large
number $M\geq M_1$ such that if  $m\geq M$,
$$
r_0f'(r_0)K(r_0)\Big(\fint_{\Omega}\frac{1}{1+r_0\rho(x)}\Big)^{-1}>1.
$$
Then for fixed large $m\geq M$, we can choose $d_1/d_2$ sufficiently
large such that  $\mu_1'(r_0)+\mu_2'(r_0)<0$. By virtue of the
expression of $\mu_1(r)+\mu_2(r)$, one sees that if $d_1/d_2$ and
$m$ are large, there exists $\bar{r}>r_0$ such that
$$\mu_1(r)+\mu_2(r)>0\quad\text{for }r\in (r_0, \bar{r}),$$
\begin{equation}\label{54}
\mu_1(\bar{r})+\mu_2(\bar{r})=0 \quad\text{and}\quad 
\mu_1'(\bar{r})+\mu_2'(\bar{r})<0.
\end{equation}


In the following, if we  find positive numbers $\xi^*$ and
$\varepsilon$ such that $\lambda_1(\xi^*, \varepsilon)$ and
$\lambda_2(\xi^*, \varepsilon)$ form a pure imaginary pair and
satisfy $\partial_{\xi}(\lambda_1(\xi^*,
\varepsilon)+\lambda_2(\xi^*, \varepsilon))<0$, then the abstract
Hopf bifurcation theorem for strongly coupled parabolic equations
from Amann \cite{amann} (see also \cite{crandall}) can deduce the
proposition. This is our step two.

 To show this, by Lemma \ref{lemma4.3}, we apply the implicit function 
theorem to construct the eigenvalue $\lambda$ and its corresponding
eigenfunction $(\phi, \psi)$ of \eqref{42} as the forms
$$
\lambda=\varepsilon \nu,\quad 
(\phi, \psi)=(1, \eta)+\varepsilon \mathbf{V}, \quad \mathbf{V}\in X_1.$$
Substituting $\lambda$ and $(\phi, \psi)$ of this form into
\eqref{42}, we obtain
$$H((1, \eta)+\varepsilon \mathbf{V})+\varepsilon
\hat{B}(\xi, \varepsilon)[(1, \eta)+\varepsilon
\mathbf{V}]+\varepsilon \nu J(\xi, \varepsilon)[(1, \eta)+\varepsilon
\mathbf{V}]=0,$$ where $\hat{B}(\xi, \varepsilon)=B_{(w,z)}(w(\xi,
\varepsilon), z(\xi, \varepsilon), \alpha(\xi, \varepsilon) )$. Then
after defining the mapping $G: \mathbb{R}^2 \times
\mathbb{C}^2\times X_1\to Y$ by
$$
G(\xi, \varepsilon, \nu, \eta, \mathbf{V})
=H((1, \eta)+\varepsilon \mathbf{V})+\varepsilon
\hat{B}(\xi, \varepsilon)[(1, \eta)+\varepsilon
\mathbf{V}]+\varepsilon \nu J(\xi, \varepsilon)[(1, \eta)+\varepsilon
\mathbf{V}],
$$ 
the eigenvalue problem \eqref{42} is equivalent to
$$
G(\xi, \varepsilon, \nu, \eta, \mathbf{V})={\bf{0}}.
$$
 We further decompose this equation as
\begin{equation}
\begin{gathered}
 (I-Q)\hat{B}(\xi, \varepsilon)[(1, \eta)+\varepsilon
\mathbf{V}]+\nu (I-Q)J(\xi, \varepsilon)[(1, \eta)+\varepsilon
\mathbf{V}]=0,\\
 QH(\mathbf{V})+Q\hat{B}(\xi, \varepsilon)[(1, \eta)+\varepsilon
\mathbf{V}]+\nu QJ(\xi, \varepsilon)[(1, \eta)+\varepsilon
\mathbf{V}]=0,
 \end{gathered}  \label{55}
 \end{equation}
where $Q: Y\to Y_1$ is the $L^2$-orthogonal projection. Then
define the mapping
$$
G^1:\mathbb{R}^2 \times \mathbb{C}^2\times
X_1\to \mathbb{R}^2
$$ 
by the left-hand side of the first
equation of \eqref{55} and
$$
G^2:\mathbb{R}^2 \times \mathbb{C}^2\times X_1\to Y_1
$$
 by the left-hand side of the second equation of
\eqref{55}.

Let $\bar{r}$ be the positive number given  above. Note that
\begin{gather*}
(I-Q)\hat{B}(\bar{r}, 0)=\Phi^0_{(r,s)}(\bar{r}, f(\bar{r}), g(\bar{r})),\\
(I-Q)J(\bar{r}, 0)=J(\bar{r}),
\end{gather*}
here $\Phi^0_{(r,s)}$ and
$J(\bar{r})$ are given in Lemma \ref{lemma4.3}. Let $\nu_1$ and
$\nu_2$ be the eigenvalues of $M(\bar{r})$ and denote $(1, \eta_1)$
and $(1, \eta_2)$ by the corresponding eigenfunctions. Note that we
can choose $d_1/d_2$ large enough such that all the entries of
$M(\bar{r})$ are nonzero, so the eigenfunctions can be of the form
$(1, \eta_i)$. Therefore,
$$
G(\bar{r}, 0, \nu_j, \eta_j, \mathbf{V}_j)={\bf{0}},
$$
with $\mathbf{V}_j=-(QH)^{-1}\left(Q\hat{B}(\bar{r}, 0)(1,
\eta_j)+\nu_j QJ(\bar{r}, 0)(1, \eta_j)\right)$ and $j=1,2$.

On the other hand,
\begin{gather*}
\begin{aligned}
&G^1_{(\nu, \eta, \mathbf{V})}(\bar{r}, 0, \nu_j, \eta_j, \mathbf{V}_j
)[\bar{\nu}, \bar{\eta}, \bar{\mathbf{V}}]\\
&=\Phi^0_{(r, s)}(\bar{r}, f(\bar{r}), g(\bar{r}))(0,
\bar{\eta})+\bar{\nu}J(\bar{r})(1, \eta_j)+\nu_j J(\bar{r})(0,
\bar{\eta}),
\end{aligned} \\
\begin{aligned}
&G^2_{(\nu, \eta, \mathbf{V})}(\bar{r}, 0, \nu_j, \eta_j, \mathbf{V}_j
)[\bar{\nu}, \bar{\eta}, \bar{\mathbf{V}}]\\
&=QH(\bar{\mathbf{V}})+Q\hat{B}(\bar{r}, 0)(0,
\bar{\eta})+\bar{\nu}QJ(\bar{r}, 0)(1, \eta_j) +\nu_j QJ(\bar{r},
0)(0, \bar{\eta}),
\end{aligned}
\end{gather*}
then \eqref{390} and $g'(\bar{r})>0$ deduce that
$\Phi^0_{(r,s)}(\bar{r}, f(\bar{r}), g(\bar{r}))$ is invertible.
Then we can also deduce that $G_{(\nu, \eta, \mathbf{V})}(\bar{r}, 0,
\nu_j, \eta_j, \mathbf{V}_j)$ is invertible. Thus, by the implicit
function theorem, the eigenvalue $\lambda_j(\xi, \varepsilon)$ of
\eqref{42} can be expressed by
$$
\lambda_j(\xi, \varepsilon)=\varepsilon \nu_j(\xi, \varepsilon)
$$
for a certain smooth function $\nu_j(\xi, \varepsilon)$ in a
neighborhood of $(\bar{r}, 0)$ for $j=1,2$. Moreover,
$\nu_j(\bar{r}, 0)=\mu_j(\bar{r})$. Then by the smoothness of the
function $\nu_j(\xi, \varepsilon)$ and \eqref{54}, we can find the
 desired $(\xi^*, \varepsilon)$. The proposition
is proved.
\end{proof}


Then, the regularity of the scaling \eqref{32} asserts Theorem
\ref{thm2.4}  in Section 3.


\subsection*{Acknowledgments}
This research was supported by: grants 11031003, 11271172, 11226153 from the 
NSF of China, grant lzujbky-2011-148 from FRFCU,  and CSC.

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\end{document}

