\documentclass[reqno]{amsart}
\usepackage{hyperref}
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\AtBeginDocument{{\noindent\small
\emph{Electronic Journal of Differential Equations},
Vol. 2017 (2017), No. 173, pp. 1--19.\newline
ISSN: 1072-6691. URL: http://ejde.math.txstate.edu or http://ejde.math.unt.edu}
\thanks{\copyright 2017 Texas State University.}
\vspace{8mm}}

\begin{document}
\title[\hfilneg EJDE-2017/173\hfil Activator-substrate model]
{Turing and Hopf bifurcation of Gierer-Meinhardt activator-substrate model}

\author[R. Wu, Y. Shao, Y. Zhou, L. Chen \hfil EJDE-2017/173\hfilneg]
{Ranchao Wu, Yan Shao, Yue Zhou, Liping Chen}

\address{Ranchao Wu \newline
School of Mathematics,
Anhui University,
Hefei 230601, China}
\email{rcwu@ahu.edu.cn}

\address{Yan Shao \newline
School of Mathematics,
Anhui University,
Hefei 230601, China}
\email{yanshao28@126.com}

\address{Yue Zhou \newline
School of Mathematics,
Anhui University,
Hefei 230601, China}
\email{zhouyue1016@126.com}

\address{Liping Chen \newline
 School of Electrical Engineering and Automation,
 Hefei University of Technology,
Hefei 230009,China}
\email{lip\_chenhut@126.com}

\dedicatory{Communicated by Zhaosheng Feng}

\thanks{Submitted October 3, 2016. Published July 10, 2017.}
\subjclass[2010]{35B36, 35B32, 37G05}
\keywords{Pattern formation; Gierer-Meinhardt model; Turing instability;
\hfill\break\indent Hopf bifurcation}

\begin{abstract}
 Gierer-Meinhardt model acts as one of prototypical reaction diffusion
 systems describing pattern formation phenomena in natural events.
 Bifurcation analysis, including theoretical and numerical analysis, is
 carried out on the Gierer-Meinhardt activator-substrate model.
 The effects of diffusion on the stability of equilibrium points and the
 bifurcated limit cycle from Hopf bifurcation are investigated.
 It shows that under some conditions, diffusion-driven instability, i.e,
 the Turing instability, about the equilibrium point will occur, which is
 stable without diffusion. While once the diffusive effects are present,
 the bifurcated limit cycle, which is the spatially homogeneous periodic
 solution and stable without the presence of diffusion, will become unstable.
 These diffusion-driven instabilities will lead to the occurrence of
 spatially nonhomogeneous solutions. Consequently, some pattern formations,
 like stripe and spike solutions, will appear. To understand the Turing
 and Hopf bifurcation in the system, we use dynamical techniques,
 such as stability theory, normal form and center manifold theory.
 To illustrate theoretical analysis, we carry out numerical simulations.
\end{abstract}

\maketitle
\numberwithin{equation}{section}
\newtheorem{theorem}{Theorem}[section]
\newtheorem{remark}[theorem]{Remark}
\allowdisplaybreaks

\section{Introduction}

Natural patterns are various in shape and form. The development processes
 of such patterns are complex, and also interesting to researchers.
To understand the underlying mechanism for patterns of plants and animals,
Turing \cite{Turing} first proposed the coupled reaction-diffusion equations.
It was showed that the stable process could evolve into an instability with
diffusive effects. He showed that diffusion could destabilize spatially
homogeneous states and cause nonhomogeneous spatial patterns, which accounted
for biological patterns in plants and animals. Such instability is frequently
called the Turing instability, also known as diffusion-driven instability.
Gierer and Meinhardt \cite{GM} presented a prototypical model of coupled
reaction diffusion equations, which described the interaction between
two substances, the activator and the inhibitor, and was used to describe the
Turing instability. The Gierer-Meinhardt model is expressed in the following form
\begin{equation}\label{e1.1}
 \begin{gathered}
 \frac{\partial a}{\partial t}=\rho_0\rho+c\rho\frac{a^{r}}{h^s}
 -\mu a+D_a \frac{\partial^2 a}{\partial x^2},\\
\frac{\partial h}{\partial t}=c'\rho'\frac{a^{T}}{h^u}
 -vh+D_h\frac{\partial^2 h}{\partial x^2}.
 \end{gathered}
 \end{equation}
where $a(x,t)$ and $h(x,t)$ represent the population densities of the activator
and the inhibitor at time $t>0$ and spatial location $x$, respectively.
$D_a$ and $D_h$ are the diffusion constants of the activator and the inhibitor,
respectively; $\rho\rho_0$ is the source concentration for the activator;
$\rho'$ is the one for the inhibitor; the activator and the inhibitor are
removed by the first order kinetics $\mu a $ and $vh$, respectively,
either by enzyme degradation, or leakage, or re-uptake by the source,
or by any combination of such mechanisms; now the sources of activator and
the inhibitor are assumed to be uniformly distributed, that is, $\rho$
and $\rho'$ are constants.

Several results about such model have been achieved. If $s\neq u$, it is
said to have different sources. If $s=u$, then it is said to be the model
with common sources. When $r=2, s=1, T=2$ and $u=0$, Ruan \cite{Ruan}
investigated the instability of equilibrium points and the periodic solutions
under diffusive effects, which were stable without diffusion.
The perturbation method was employed to carry out the analysis there.
In \cite{Gonpot}, they showed the analysis of the Turing instability for such model. By using the bifurcation technique, Liu et al. \cite{LiuWei} obtained the results about the Hopf bifurcation, the steady state bifurcation and their interaction in this model. However, the model was subject to fixed Dirichlet boundary conditions. Recently, Song \cite{song} further investigated the Turing-Hopf bifurcation and spatial resonance phenomena in this model. When $r=2, s=2, u=0,T=1$ and $u=0$, Wang et al. \cite{WangJL} studied the Turing instability and the Hopf bifurcation.

Also, the Turing instability for the semi-discrete Gierer-Meinhardt model
 was considered in \cite{DiscreteGM}. Bifurcation for the Gierer-Meinhardt
model with saturation was analyzed in \cite{GMsaturation}. The influence
of gene expression time delay on the patterns of Gierer-Meinhardt system
was explored in \cite{DelayGM}. The Turing bifurcation in models like
Brusselator and Gierer-Meinhardt systems were analyzed in \cite{Dilao}.

The existence, asymptotic behaviors of solutions and their stability
in terms of diffusion effects have been extensively investigated,
for example, \cite{Ni,Veerman,Blowup,Zou,WeiJC} and references therein.

In view of the processes in morphogenesis, which was described in detail
in \cite{GM}, if it is assumed that the sources of distribution are activated
by $a(x, t)$ and further by some substance of concentration $s(x, t)$,
one could give the activator-substrate (depletion) model. Here, the
 substance of concentration $s(x, t)$ could be consumed by activation or
some indirect effect of activation. In one dimension, the depletion model
could be written as follows
\begin{equation}\label{e1.2}
\begin{gathered}
 \frac{\partial a}{\partial t}= a^2h-\mu a
+D_a\frac{\partial^2 a}{\partial x^2},\\
\frac{\partial h}{\partial t}=c_0-c'\rho a^2h-vh
+D_h\frac{\partial^2 h}{\partial x^2}.
 \end{gathered}
 \end{equation}
This model was used to describe pigmentation patterns in sea shells
\cite{Klingler,Buceta} and the ontogeny of ribbing
on ammonoid shells \cite{Hammer}. By means of qualitative analysis,
such as stability theory, normal form and bifurcation technique,
we will investigate the Turing instability of the system with Neumann
 boundary conditions. Furthermore, some patterns will be identified numerically.

By using the scaling transformation, let
\[
t=\frac{\tau}{v},\quad \bar{\mu}=\frac{\mu}{v},\quad
D_{H}=\frac{D_h}{v},\quad D_{A}=\frac{D_a}{v},
\]
then one has
\begin{gather*}
\frac{\partial A}{\partial \tau}=A^2 H-\bar{\mu}A
+D_A\frac{\partial^2 A}{\partial x^2},\\
\frac{\partial H}{\partial \tau}=c_0-A^2H-H
+D_H\frac{\partial^2 H}{\partial x^2}.
\end{gather*}
For simplicity, we change parameters $ A,H,\tau,\bar{\mu},c_0,D_{A},D_{H}$
into $ a,h,t,\mu,c,D_{a},D_{h} $, respectively.
System \eqref{e1.2} can be written as follows
\begin{equation} \label{e1.3}
\begin{gathered}
\frac{\partial a}{\partial t}=a^2h-\mu a+D_a\frac{\partial^2 a}{\partial x^2},\\
\frac{\partial h}{\partial t}=c-a^2h-h+D_h\frac{\partial^2 h}{\partial x^2}.\\
\end{gathered}
\end{equation}
where $\mu,c,D_{a},D_{h}>0,a,h\geq0$. In the sequel, system \eqref{e1.3}
is assumed to be subjected to the Neumann boundary conditions
$$
\frac{\partial{a}}{\partial{x}}(0,t)=\frac{\partial{a}}
{\partial{x}}(\pi,t)=0,\quad
\frac{\partial{h}}{\partial{x}}(0,t)=\frac{\partial{h}}{\partial{x}}(\pi,t)=0.
$$

\section{Analysis of system without diffusion}

When the diffusive terms in system \eqref{e1.3} are absent, it will reduce
to the local system
\begin{equation} \label{e2.1}
\begin{gathered}
\frac{da}{dt}=a^2h-\mu a,\\
\frac{dh}{dt}=c-a^2h-h.\\
\end{gathered}
\end{equation}
Let
$$
f(a,h)=a^2h-\mu a,~~~~g(a,h)=c-a^2h-h.
$$

Let $l=\frac{c}{\mu}$. Note that if $0<l<2$, system \eqref{e2.1}
has a unique equilibrium point $S(0, c)$; if $l=2$, the system
has equilibrium points $S$ and $P^*(1, \mu)$; if $l>2$, it has
equilibrium points $S$,
\[
P_0\Big(\frac{l+\sqrt{l^2-4}}{2}, \frac{l-\sqrt{l^2-4}}{2}\mu\Big),\quad
P_1\Big(\frac{l-\sqrt{l^2-4}}{2}, \frac{l+\sqrt{l^2-4}}{2}\mu\Big).
\]
 In fact, when $l=2$, $P_0$ and $P_1$ will coincide to be the
point $P^*(1, \mu)$.

The Jacobian matrix of \eqref{e2.1} evaluated at the equilibrium point $S$ is
\[
J(S)=\begin{pmatrix}
 -\mu & 0 \\
 0 & -1
\end{pmatrix},
\]
so $S$ is the asymptotically stable node.

The Jacobian matrix of \eqref{e2.1} evaluated at the equilibrium point $P_1$ is
\[
J(P_1)=\begin{pmatrix}
 \mu & \frac{l^2-l\sqrt{l^2-4}-2}{2} \\
 -2\mu & -\frac{l^2-l\sqrt{l^2-4}}{2}
\end{pmatrix}.
\]
Then $\operatorname{tr}(J)=\mu-\frac{l^2-l\sqrt{l^2-4}}{2}$,
$\det(J)=\frac{\mu}{2}\sqrt{l^2-4}(\sqrt{l^2-4}-l)<0$, so $P_1$
 is the unstable saddle.

From the above analysis about the existence and stability of equilibrium points,
one has the following result.

\begin{theorem} \label{thm2.1}
 The equilibrium point $S$ is the asymptotically stable node.
When $0<l<2$, system \eqref{e2.1} only has the equilibrium point $S$. When $l>2$,
two other equilibrium points $P_0$ and $P_1$ will appear.
The point $P_1$ is the unstable saddle.
\end{theorem}



\begin{remark} \label{rmk2.1}\rm
 From the later analysis, note that when diffusion effect is taken into
consideration, $S$ will still be stable and $P_1$ will still be unstable.
Thus, no Turing instability will occur at these points. Next the dynamical
behaviors of $P_0$ without diffusion will be given.
\end{remark}


The Jacobian matrix of \eqref{e2.1} evaluated at the equilibrium point $P_0$ is
\[
J(P_0)=\begin{pmatrix}
 \mu & \frac{l^2+l\sqrt{l^2-4}-2}{2} \\
 -2\mu & -\frac{l^2+l\sqrt{l^2-4}}{2}
\end{pmatrix}.
\]
Note that the corresponding characteristic equation for $J(P_0)$ is
\begin{align}\label{e2.2}
\lambda^2-\operatorname{tr}(J(P_0))\lambda+DetJ(P_0)=0,
\end{align}
where $\operatorname{tr}(J(P_0))=\mu-\frac{l(l+\sqrt{l^2-4})}{2}$ and
$\det J(P_0)=\frac{\mu[l^2+l\sqrt{l^2-4}-4]}{2}>0$.



\begin{theorem} \label{thm2.2}
The equilibrium point $P_0$ of system \eqref{e2.1} is asymptotically stable if
\begin{equation} \label{H1}
 \mu<\frac{l(l+\sqrt{l^2-4})}{2}
\end{equation}
and is unstable if
\begin{equation} \label{H2}
\mu>\frac{l(l+\sqrt{l^2-4})}{2}.
\end{equation}
\end{theorem}

\begin{proof}
If \eqref{H1} holds, then the eigenvalues are both negative or have negative 
real parts, so the equilibrium $P_0$ of \eqref{e2.1} is stable;
if \eqref{H2} holds, then the eigenvalues are both positive or have positive
 real parts, so the equilibrium $P_0$ of \eqref{e2.1} is unstable.
\end{proof}


From Theorem \ref{thm2.2}, we know that the Hopf bifurcation may occur at the point 
$P_0$ in system \eqref{e2.1}. Next the Hopf bifurcation at the point $P_0$ and
its direction will be investigated. For simplicity, let 
$\mu_0=\frac{l(l+\sqrt{l^2-4})}{2}$ and $(a_0, h_0)$ denote the point $P_0$.
In terms of the characteristic equation \eqref{e2.2}, the eigenvalues are
\[
 \lambda_1,_2=\frac{\operatorname{tr}(J)
\pm\sqrt{\operatorname{tr}(J)^2-4\det(J)}}{2}.
\]

 If $\operatorname{tr}(J)^2<4\det(J)$, then it has a pair of complex roots,
 with real parts $\frac{\operatorname{tr}(J)}{2}$.
 Note that $\frac{dRe\lambda_1,_2}{d\mu}|_{\mu_0}=1>0$,
thus the Hopf bifurcation may occur in system \eqref{e2.1} when $\mu=\mu_0$.
The Hopf bifurcation curve is defined by $\operatorname{tr}(J)=0$, i.e.,
\[
\mu=\frac{l(l+\sqrt{l^2-4})}{2}.
\]
As for the direction of Hopf bifurcation, it could be derived as the way 
in \cite{Wiggins} as follows.
Let $a\to a+a_0, h\to h+h_0$, so
\begin{equation} \label{e2.3}
\begin{pmatrix}
\frac{da}{dt}\\
\frac{dh}{dt}
\end{pmatrix}
=\begin{pmatrix}
f(a_0+a,h_0+h) \\
g(a_0+a,h_0+h)
\end{pmatrix}
 = J(P_0)\begin{pmatrix}
 a\\
 h
\end{pmatrix} 
+ \begin{pmatrix}
 f_2(a,h) \\
 g_2(a,h)
\end{pmatrix},
\end{equation}
where
\[
f_2(a,h,\mu)=a^2 h_0+2a_0ah+a^2 h,~
g_2(a,h,\mu)=-a^2h_0-2a_0ah-a^2h.
\]

When $\mu=\mu_0$, we verify that $\lambda_1,_2(\mu_0)=\pm i\omega_0$,
 where $\omega_0^2=\frac{\mu[l^2+l\sqrt{l^2-4}-4]}{2}>0$.
We choose one of eigenvectors corresponding to the eigenvalue
$i\omega_0$ of matrix $J(P_0)$ at $\mu=\mu_0$ to be $\xi=(i\omega_0+\mu,-2\mu)^{T}$.
Let
\[
T= \begin{pmatrix}
 \omega_0 & \mu\\
 0 & -2\mu
 \end{pmatrix},
\]
then
\[
T^{-1}= \begin{pmatrix}
 \frac{1}{\omega_0} & \frac{1}{2\omega_0} \\
 0 & -\frac{1}{2\mu} 
 \end{pmatrix}.
\]
The transformation $ \begin{pmatrix}
 a \\
 h \\
 \end{pmatrix}
= P \begin{pmatrix}
 u \\
 v \\
 \end{pmatrix}$
 changes \eqref{e2.1} into
\begin{align*}
\begin{pmatrix}
 \frac{du}{dt} \\
 \frac{dv}{dt}
 \end{pmatrix}
&=P^{-1}JP\begin{pmatrix}
 u \\
 v 
 \end{pmatrix}
 +P^{-1} \begin{pmatrix}
 f_2P(u,v) \\
 g_2P(u,v) 
 \end{pmatrix}\\
 &= \begin{pmatrix}
 0 & -\omega_0 \\
 \omega_0 & 0 
 \end{pmatrix}
  \begin{pmatrix}
 u \\
 v 
 \end{pmatrix}
 + \begin{pmatrix}
 f_3(u,v) \\
 g_3(u,v)
 \end{pmatrix},
\end{align*}
where
\begin{gather*}
\begin{pmatrix}
 f_3(u,v) \\
 g_3(u,v)
 \end{pmatrix}
= \begin{pmatrix}
 \frac{1}{2\omega_0}f_2(\omega_0u+\mu v,-2\mu v) \\
 -\frac{1}{2\mu}g_2(\omega_0u+\mu v,-2\mu v) 
 \end{pmatrix}, \\
\begin{aligned}
f_2(\omega_0u+\mu v,-2\mu v)
&= \omega_0^2u^2h_0+\mu^2v^2h_0+2\omega_0\mu huv-4a_0\omega_0\mu uv\\
&\quad -4a_0\mu^2v^2-2\mu\omega_0^2u^2v-2\mu^{3}v^{3}-4\omega_0\mu^2uv^2,
\end{aligned}\\
g_2(\omega_0u+\mu v,-2\mu v)=-f_2(\omega_0u+\mu v,-2\mu v).
\end{gather*}
Then 
\begin{gather*}
f_{2uu}=2h_0\omega_0^2-4\mu\omega_0^2v, \quad
 f_{2uuv}=-4\mu\omega_0^2,\quad f_{2uuu}=0,\\
f_{2uv}=2\omega_0\mu h_0-4a_0\mu\omega_0,\quad
f_{2uvv}=-8\mu^2\omega_0,\quad f_{2vv}=2\mu^2h_0-8a_0\mu^2,\\
g_{2uu}=-2h_0\omega_0^2+4\mu\omega_0^2v,\quad g_{2vvv}=12\mu^{3},\quad
g_{2uuu}=0,\\
g_{2uv}=-2\omega_0\mu h_0+4a_0\mu\omega_0,\quad g_{2uvv}=8\mu^2\omega_0,\quad
g_{2vv}=-2\mu^2h_0+8a_0\mu^2.
\end{gather*}
So the stability of Hopf bifurcation in system \eqref{e2.1} at $P_0(a_0,h_0)$ 
is determined by the sign of the following quantity  \cite{Wiggins}
\begin{align*}
 \sigma&=\frac{1}{16}(f_{3uuu}+g_{3uuv}+f_{3uvv}+g_{3vvv})\\
 &\quad +\frac{1}{16\omega_0}[f_{3uv}(f_{3uu}+f_{3vv})-g_{3uv}
 (g_{3uu}+g_{3vv})-f_{3uu}g_{3uu}+f_{3vv}g_{3vv}],
\end{align*}
where all the partial derivatives are evaluated at the bifurcation point 
$(u,v,\mu)=(0,0,\mu_0)$.

We can find that
\begin{gather*}
f_{3uu}=h\omega_0,\quad f_{3uuu}=0,\quad f_{3uv}=\mu h-2a\mu,\quad f_{3uvv}=-4\mu^2,\\
f_{3vv}=\frac{\mu^2h-4a\mu^2}{\omega_0}, \quad g_{3uu}=\frac{h\omega_0^2}{\mu},
\quad g_{3uuv}=-2\omega_0^2,\\
g_{3uv}=\omega_0 h-2a\omega_0,\quad g_{3vv}=\mu h-4a\mu,\quad g_{3vvv}=-6\mu^2,
\end{gather*}
then
\[
\sigma=\frac{-\omega_0^{4}(2\mu+h^2)-\mu^{3}[10\omega_0^2-2(h-2a)
(-l-\sqrt{l^2-4})-\mu(h-4a)^2]}{16\omega_0^2\mu}
 <0.
\]
From the above analysis, one has the the following Hopf bifurcation 
result at the point $P_0$.

\begin{theorem} \label{thm2.3}
When $\operatorname{tr}(J)^2<4\det(J)$, system \eqref{e2.1} undergoes 
a supercritical Hopf bifurcation at $\mu=\mu_0$ and
the bifurcated limit cycle is stable as $\mu>\mu_0$.
\end{theorem}

For an illustration of the Hopf bifurcation, see Figures \ref{fig1} and \ref{fig2}.

\begin{figure}[htb] 
\begin{center}
 \includegraphics[width=0.48\textwidth]{fig1} 
\end{center}
\caption{Equilibrium point $P_0$ is a stable focus.}
\label{fig1}
\end{figure}

\begin{figure}[htb] 
\begin{center}
 \includegraphics[width=0.48\textwidth]{fig2} 
\end{center}
\caption{A stable limit cycle is bifurcated from Hopf bifurcation.}
\label{fig2}
\end{figure}

When $l=2$, the equilibrium points 
\[
P_0\Big(\frac{l+\sqrt{l^2-4}}{2},\frac{l-\sqrt{l^2-4}}{2}\mu\Big),\quad
P_1\Big(\frac{l-\sqrt{l^2-4}}{2}, \frac{l+\sqrt{l^2-4}}{2}\mu\Big),
\]
with  $(l>2)$, 
coincide to be the point $P^*(1,\mu)$. The Jacobian matrix evaluated
at $P^*$ is
\[
J(P^*)=\begin{pmatrix}
  \mu & 1 \\
 -2\mu &-2
\end{pmatrix}.
\]
The corresponding eigenvalues are $\lambda_{1}=0$, $\lambda_2=\mu-2$ and
$\operatorname{tr}(J(P^*))=\mu-2$, $\det(J(P^*))=0$. So it is nonhyperbolic.
 When $\mu \neq 2$, its stability could be analyzed in the
following by employing center manifold reduction theory in \cite{Wiggins}.

Let $a\to a+1$, $h \to h+\mu$, system \eqref{e2.1} becomes
\begin{equation}
\begin{pmatrix}
 \frac{da}{dt} \\
 \frac{dh}{dt}
\end{pmatrix}
= J(P^*)\begin{pmatrix}
 a \\
 h
\end{pmatrix} + \begin{pmatrix}
 {f_2(a,h)} \\
 {g_2(a,h)}
\end{pmatrix},
\end{equation}
where
\begin{gather*}
f_2(a,h,\mu)=a^2 \mu+2ah+a^2 h,\\
g_2(a,h,\mu)=-a^2\mu-2ah-a^2h.
\end{gather*}
The Jacobian matrix at $P^*$ can be diagonalized as
\[
T^{-1}J(P^*)T=\begin{pmatrix}
  0 & 0 \\
  0 & \mu-2
\end{pmatrix},
\]
where
\[
T=\begin{pmatrix}
  1 & 1 \\
  -\mu & -2
\end{pmatrix},\quad
T^{-1}=\begin{pmatrix}
  \frac{-2}{\mu-2} &\frac{-1}{\mu-2} \\
  \frac{\mu}{\mu-2}& \frac{1}{\mu-2}
\end{pmatrix}.
\]
Consequently, the system will be changed into
\begin{equation} \label{e2.5}
\begin{aligned}
 \begin{pmatrix}
 \frac{du}{dt} \\
 \frac{dv}{dt}
 \end{pmatrix}
 &= \begin{pmatrix}
  0 & 0 \\
  0 & \mu-2
 \end{pmatrix}
 \begin{pmatrix}
 u \\
 v
 \end{pmatrix} \\
&\quad +\begin{pmatrix}
 -\frac{1}{\mu-2}(u+v)[(u+v)\mu-(\mu u+2v)(u+v+2)] \\
 \frac{\mu-1}{\mu-2}(u+v)[(u+v)\mu-(\mu u+2v)(u+v+2)]
 \end{pmatrix}.
\end{aligned}
\end{equation}
Its local center manifold at the origin can be represented as
$$
W^{c}(0)=\{(u,v)\in R^2\mid v=\gamma (u),\mid u\mid<\delta,
\gamma(0)=D\gamma(0)=0\},
$$
for $ \delta>0 $ sufficiently small. Assume that $\gamma(x)$ takes the form
\begin{equation}
 \gamma(u)=u^2+bu^{3}+O(u^{4}).
\end{equation}
Substituting it into system \eqref{e2.5} and equating coefficients on each
power of $x$ to zero, we have
\[
a=\frac{\mu(\mu-1)}{(\mu-2)^2}, \quad
b=\frac{\mu^2(\mu+2)(\mu-1)}{(\mu-2)^4},
\]
thus
\[
\gamma(u)=\frac{\mu(\mu-1)}{(\mu-2)^2}u^2
+\frac{\mu^2(\mu+2)(\mu-1)}{(\mu-2)^4}u^3+O(x^4).
\]
As a result, system \eqref{e2.5} restricted to the local center manifold is
\[
\dot u= \frac{\mu}{\mu-2} u^2+O(u^3),
\]
from which we know that the origin is unstable, that is, the point
$P^*$ is unstable.

\section{Turing instability induced by diffusion}

 When the diffusive effects are considered, it is desirable to know how the 
diffusive terms affect the stability of fixed  points and the bifurcated limit cycle.
 If the stable equilibrium points and stable limit cycles become unstable under such
 effects, then it is often known as the Turing instability, namely, the 
diffusion-driven instability. In this section,
 instability induced by diffusive effects on the equilibrium points and the 
bifurcated limit cycle will be investigated.

\subsection{Turing instability of the equilibrium points}
 Let $u=a-a_0,v=h-h_0$, then the linearized system of \eqref{e1.3} at 
$(a_0,h_0)$ is
\begin{equation} \label{e3.1}
 \begin{pmatrix}
 \frac{du}{dt} \\
 \frac{dv}{dt}
 \end{pmatrix}
= \begin{pmatrix}
 2a_0h_0-\mu+D_{a}\frac{\partial^2 }{\partial x^2} & a_0^2 \\
 -2a_0h_0 & -a_0^2-1+D_h\frac{\partial^2}{\partial x^2} \\
 \end{pmatrix}
\begin{pmatrix}
 u \\
 v
 \end{pmatrix}
=: \begin{pmatrix}
 u \\
 v
 \end{pmatrix},
\end{equation}
 with the Neumann boundary condition
\begin{equation} \label{e3.2}
 u_x(0,t)=v_x(0,t)=u_x(\pi,t)=v_x(\pi,t)=0.
\end{equation}
System \eqref{e3.1}-\eqref{e3.2} has the solution $(u,v)$ formally described as
\begin{equation}
\begin{pmatrix}
 u(x,t) \\
 v(x,t)
 \end{pmatrix}
=\sum^\infty_{k=0} \begin{pmatrix}
 a_k \\
 b_k
 \end{pmatrix}
e^{\lambda t}\cos kx.
\end{equation}
Substituting this into \eqref{e3.1}, we have
\begin{align*}
&\sum^\infty_{k=0} \begin{pmatrix}
 a_k \\
 b_k
 \end{pmatrix}\lambda e^{\lambda t}\cos kx \\
&= L(P_0) \begin{pmatrix}
 u \\
 v
 \end{pmatrix} \\
&=\sum^\infty_{k=0}
 \begin{pmatrix}
 \mu+D_{a}\frac{\partial^2 }{\partial x^2} & \frac{l^2+l\sqrt{l^2-4}-2}{2} \\
 -2\mu & -\frac{l^2+l\sqrt{l^2-4}}{2}+D_{h}\frac{\partial^2 }{\partial x^2}
 \end{pmatrix}
  \begin{pmatrix}
 a_k \\
 b_k
 \end{pmatrix}
e^{\lambda t}\cos kx.
 \end{align*}
Comparing the equal powers of $k$, we have
\begin{equation} \label{e3.4}
(\lambda I-J_k(\mu))
 \begin{pmatrix}
 a_k \\
 b_k
 \end{pmatrix}
= \begin{pmatrix}
 0 \\
 0
 \end{pmatrix}, \quad k=0,1,2,\dots,
\end{equation}
where
\[
J_k(\mu)= \begin{pmatrix}
 \mu-k^2D_{a} & \frac{l^2+l\sqrt{l^2-4}-2}{2} \\
 -2\mu & -\frac{l^2+l\sqrt{l^2-4}}{2}-k^2D_{h}
 \end{pmatrix}.
\]
So system \eqref{e3.4} has a nonzero solution $(a_k,b_k)^{T}$ if and only if
\begin{align*}
\det(\lambda I-J_k(\mu))=0.
\end{align*}
Which is the characteristic equation of the original system \eqref{e1.3} at $P_0$.
Rewrite it as the equation
\begin{equation} \label{e3.5}
\lambda^2-\operatorname{tr}(k)\lambda+\det(k)=0,
\end{equation}
where
\begin{gather*}
\operatorname{tr}(k)=\mu-\frac{l^2+l\sqrt{l^2-4}}{2}-k^2(D_{a}+D_{h})
=\operatorname{tr}(J(P_0))-k^2(D_{a}+D_{h}),\\
\begin{aligned}
\det(k)&=\frac{l^2+l\sqrt{l^2-4}-4}{2}\mu-\mu k^2D_{h}
 +\frac{l^2+l\sqrt{l^2-4}}{2}k^2D_{a}+k^4D_{a}D_{h}\\
&=k^2 D_{h}[k^2D_{a}-\mu D_{h}]+\frac{l^2+l\sqrt{l^2-4}}{2}k^2D_{a}+\det(J(P_0)).
\end{aligned}
\end{gather*}
Under condition \eqref{H1}, one has $\operatorname{tr}(k)<0$ for all $k=0,1,2,\dots$
and $\det(0)=\det(J(P_0))>0$.
Let
\begin{align*}
r_{m}=\min_{1\leq k\leq m}\frac{\det(J)+\frac{l^2+l\sqrt{l^2-4}}
{2}D_{a}k^2}{(\mu-D_{a}k^2)k^2}.
\end{align*}

If $\frac{\mu}{D_{a}}\leq1$ or $m^2<\frac{\mu}{D_{a}}\leq(m+1)^2$, and $r<r_{m}$,
then $\det(k)\geq \det(0)>0$, so $(a_0,h_0)$ is linearly asymptotically stable 
for system \eqref{e1.3}; if $m^2<\frac{\mu}{D_{a}}\leq(m+1)^2$ and $D_h>r_{m}$,
then there exists at least one negative in $\det(1),\dots,\det(m)$,
and so $(a_0,h_0)$ is unstable for system \eqref{e1.3}.
Hence, the above analysis can be summarized as follows.

\begin{theorem} \label{thm3.1}
Assume that condition \eqref{H1} holds, let
\[
r_{m}=\min_{1\leq k\leq m}\frac{\det(J)
+\frac{l^2+l\sqrt{l^2-4}}{2}D_{a}k^2}{(\mu-D_{a}k^2)k^2},
\]
then $(a_0,h_0)$ is a stable equilibrium for \eqref{e1.3} if either 
\begin{equation} \label{H3}
 \frac{\mu}{D_{a}}\leq1,
\end{equation}
or
\begin{equation} \label{H4}
m^2<\frac{\mu}{D_{a}}\leq(m+1)^2\quad\text{and}\quad D_h<r_{m}
\end{equation}
hold.
Also $(a_0,h_0)$ is an unstable equilibrium for \eqref{e1.3} if
\begin{equation} \label{H5}
 m^2<\frac{\mu}{D_{a}}\leq(m+1)^2\quad\text{and}\quad D_h>r_{m}.
\end{equation}
\end{theorem}


\begin{remark} \label{rmk3.1}\rm
 (1) At the point $S$, the characteristic equation \eqref{e3.5} changes into
\begin{equation}
\lambda^2-\operatorname{tr}(k)\lambda+\det(k)=0,
\end{equation}
where 
\begin{gather*}
\operatorname{tr}(k)=-\mu-1-k^2(D_{a}+D_{h})
=\operatorname{tr}(J(s))-k^2(D_{a}+D_{h}),\\
\begin{aligned}
\det(k)&=\mu+k^2(D_a+\mu D_{h})+k^4D_{a}D_{h}\\
&=\det(J(S))+k^2(D_a+\mu D_{h})+k^4D_{a}D_{h}.
\end{aligned}
\end{gather*}
Note that in this case $\operatorname{tr}(k)<0$ and $\det(k)>0$, 
for all $k=0, 1, 2, \dots$, so the point $S$ is still stable under 
diffusive effects.

(2) At the point $P_1$, the characteristic equation \eqref{e3.5} changes into
\begin{equation}
\lambda^2-\operatorname{tr}(k)\lambda+\det(k)=0,
\end{equation}
where
\begin{gather*}
\operatorname{tr}(k)=\mu-\frac{l^2-l\sqrt{l^2-4}}{2}-k^2(D_{a}+D_{h})\\
=\operatorname{tr}(J(P_1))-k^2(D_{a}+D_{h}),\\
\begin{aligned}
\det(k)&=\frac{l^2-l\sqrt{l^2-4}-4}{2}\mu-\mu k^2D_{h}
 +\frac{l^2-l\sqrt{l^2-4}}{2}k^2D_{a}+k^4D_{a}D_{h}\\
&=\det(J(P_1))-\mu k^2D_{h}+\frac{l^2-l\sqrt{l^2-4}}{2}k^2D_{a}+k^4D_{a}D_{h}.
\end{aligned}
\end{gather*}
Note that $\det(0)=\det(J(P_1))<0$, so the point $P_1$ is still unstable 
under diffusive effects.

(3) At the point $P^*(1, \mu)$, the characteristic equation \eqref{e3.5} 
changes into
\begin{equation}
\lambda^2-\operatorname{tr}(k)\lambda+\det(k)=0,
\end{equation}
where
\begin{gather*}
\operatorname{tr}(k)=\mu-2-k^2(D_{a}+D_{h})
=\operatorname{tr}(J(P^*))-k^2(D_{a}+D_{h}),\\
\det(k)=-\mu k^2D_{h}+2k^2D_{a}+k^4D_{a}D_{h}.
\end{gather*}

Note that $\operatorname{tr}(0)=\mu-2, \det(0)=\det(J(P^*))=0$, 
from the previous analysis, it is unstable $(\mu\neq 2)$. So the point 
$P^*$ is still unstable under diffusive effects, from analysis of the 
Turing and Hopf interaction in \cite{Interaction}.
\end{remark}



\subsection{Turing instability of the bifurcated limit cycle}

To analyze the effects induced by diffusion on the stability of the bifurcated 
limit cycle, we apply the center manifold reduction and normal form
technique to system \eqref{e1.3}. From the first nonvanishing coefficient 
of Poincar\'{e} normal form, combined with the eigenvalues
of linearized system at the point $P_0$ and the bifurcation value $\mu_0$, 
the stability of the bifurcated limit cycle could be identified.
To this end, some necessary transformation procedures and analysis about 
the eigenvalues will be carried out.

Let $\mu=\mu_0$ and take the transformation~$u=a-a_0,~v=h-h_0,~U=(u,v)^{T}$, 
so system \eqref{e1.3} can be rewritten as
\begin{equation} \label{e3.9}
\begin{gathered}
 U_t=\Big[ J({\mu _0)+ \begin{pmatrix}
 D_a \partial _{xx} &0 \\
 0 & D_h \partial _{xx}
\end{pmatrix} \Big]U + F(U,{\mu _0})} ,\\
 U_x(0,t)=U_x(\pi ,t) = (0,0)^T,
\end{gathered}
\end{equation}
where
\[
F(U,\mu_0)=(f_2(u,v,\mu_0),(g_2(u,v,\mu_0))^{T},
\]
$f_2$ and $g_2$ are defined in \eqref{e2.3}. As in \cite{Hassard}, $F(U,\mu_0)$
can be rewritten into
\begin{align*}
F(U,\mu_0)=\frac{1}{2}Q(U,U)+\frac{1}{6}C(U,U,U)+O(|U|^{4})
\end{align*}
and
\[
Q(U,V)=\begin{pmatrix}
 Q_{1}(U,V) \\
 Q_2(U,V)
 \end{pmatrix},\quad
C(U,V,W)=\begin{pmatrix}
 C_{1}(U,V,W) \\
 C_2(U,V,W)
 \end{pmatrix},
\]
so
\begin{gather*}
\begin{aligned}
Q_1(U,V)
&=f_{2uu}u_1v_1+f_{2uv}u_1v_2+f_{2vu}u_2v_1+f_{2vv}u_2v_2\\
&=2(h_0u_{1}v_{1}+a_0u_{1}v_2+au_2v_{1}),
\end{aligned} \\
\begin{aligned}
Q_2(U,V)
&=g_{2uu}u_{1}v_{1}+g_{2uv}u_{1}v_2+g_{2vu}u_2v_{1}+g_{2vv}u_2v_2\\
&=-Q_1(U,V),
\end{aligned} \\
\begin{aligned}
C_{1}(U,V,W)
&=f_{2uuu}u_{1}v_{1}w_{1}+f_{2uuv}u_{1}v_{1}w_2+f_{2uvu}u_{1}v_2w_{1}
 +f_{2uvv}u_{1}v_2w_2 \\
&\quad +f_{2vuu}u_2v_{1}w_{1}+f_{2vuv}u_2v_{1}w_2+f_{2vvu}u_2v_2w_{1}
 +f_{2vvv}u_2v_2w_2\\
&=2(u_{1}v_{1}w_2+u_{1}v_{1}w_{1}+u_2v_{1}w_{1}),
\end{aligned} \\
\begin{aligned}
C_2(U,V,W)
&=g_{2uuu}u_{1}v_{1}w_{1}+g_{2uuv}u_{1}v_{1}w_2+g_{2uvu}u_{1}v_2w_{1}
 +g_{2uvv}u_{1}v_2w_2\\
&\quad +g_{2vuu}u_2v_{1}w_{1}+g_{2vuv}u_2v_{1}w_2+g_{2vvu}u_2v_2w_{1}
 +g_{2vvv}u_2v_2w_2\\
&=-C_{1}(U,V,W),
\end{aligned}
\end{gather*}
for any $U=(u_{1},u_2)^{T}$, $V=(v_{1},v_2)^{T}$, $W=(w_{1},w_2)^{T}$,
and $U$, $V$, $W$ $\in  H^2([0,\pi])\times  H^2([0,\pi])$.
For $\mu=\mu_0$, the linear operator $L=L(\mu_0)$ is defined by
\[
LU = \Big[ J(\mu _0)+\begin{pmatrix}
 D_a \partial _{xx} &0 \\
 0& D_h \partial _{xx}
\end{pmatrix} \Big]U
\]
and let $L^{*}$ be the adjoint operator of $L$, then
\[
L^{*}U = \Big[ J^{*}({\mu _0})+\begin{pmatrix}
 D_a \partial _{xx} &0 \\
 0&D_h \partial _{xx}
\end{pmatrix} \Big]U,
\]
with
\begin{gather*}
J(\mu_0)=\begin{pmatrix}
 \frac{l^2+l\sqrt{l^2-4}}{2} & \frac{l^2+l\sqrt{l^2-4}-2}{2} \\
 -(l^2+l\sqrt{l^2-4}) & -\frac{l^2+l\sqrt{l^2-4}}{2}
\end{pmatrix},\\
J^{*}(\mu_{_0})=\begin{pmatrix}
 \frac{l^2+l\sqrt{l^2-4}}{2} & -(l^2+l\sqrt{l^2-4}) \\
 \frac{l^2+l\sqrt{l^2-4}-2}{2} & -\frac{l^2+l\sqrt{l^2-4}}{2}
 \end{pmatrix}.
\end{gather*}

Clearly, $\langle L^{*}U,V \rangle = \langle U,LV \rangle$ for any 
$U,V\in H^2([0,\pi])\times H^2([0,\pi])$
and the inner product in $ H^2([0,\pi])\times  H^2([0,\pi])$ is defined as 
$\langle U,V\rangle  = \frac{1}{\pi}\times \int^{\pi}_0\overline{U}^{T}Vdx$
for any $U, V\in H^2([0,\pi]) \times H^2([0,\pi])$.
The linearized system of \eqref{e3.9} at the equilibrium $(0,0)$ is
\begin{equation} \label{e3.10}
U_t = LU
\end{equation}
with the Neumann boundary condition
\begin{equation} \label{e3.11}
U_x(0,t) = U_x(0,t) = (0,0)^{T}.
\end{equation}

System \eqref{e3.10} with boundary condition \eqref{e3.11} has a solution
 that can be formally represented as
\begin{equation} \label{e3.12}
U=\sum_{k=0}^{\infty}\begin{pmatrix}
 a_k \\
 h_k
 \end{pmatrix} e^{\lambda t}\cos kx,
\end{equation}
where $a_k$ and $h_k$ are complex numbers, $k$ is the wave number $k=0,1,2\dots$,
and $\lambda$ $\in$ $\mathbf{C}$ is the temporal spectrum.
Substituting \eqref{e3.12} into \eqref{e3.9} and collecting the like terms
about $k$, one has
\begin{equation} \label{e3.13}
(\lambda I-L_k)\begin{pmatrix}
 a_k \\
 h_k
 \end{pmatrix}=\begin{pmatrix}
 0 \\
 0
 \end{pmatrix},\quad  k=0,1,2,\dots,
\end{equation}
where
\[
L_k = \begin{pmatrix}
 \frac{l^2+l\sqrt{l^2-4}}{2}-D_{a}k^2 & \frac{l^2+l\sqrt{l^2-4}-2}{2} \\
 -(l^2+l\sqrt{l^2-4}) & -\frac{l^2+l\sqrt{l^2-4}}{2}-D_{h}k^2
 \end{pmatrix}.
\]

For some $k$, Equation \eqref{e3.13} has a nonzero solution $(a_k,h_k)^{T}$ 
if and only if the dispersion relation is satisfied,
$\det(\lambda I - L_k) = 0$. 
From such dispersion relation, the characteristic equation follows immediately
\begin{equation}
\lambda^2-\operatorname{tr}(L_k)+\det(k) =0, \quad k = 0,1,2,\dots,
\end{equation}
where
\begin{gather*}
\operatorname{tr}(L_k)=-(D_{a}+D_{h})k^2,\\
\det(L_k)= D_{h}k^2(D_{a}k^2-\frac{l^2+l\sqrt{l^2-4}}{2})
 +D_{a}k^2\frac{l^2+l\sqrt{l^2-4}}{2}+\det(J).
\end{gather*}


Note that when $\mu = \mu_0$, one has $\operatorname{tr}(L_0)=0$, 
$\det(L_0)=\det(J)=\mu_0(\mu_0-2) > 0$, $\operatorname{tr}(L_k) < 0$ for 
$k=1,2,\dots$.
Then for $k=0$, $L$ has eigenvalues with zero real parts, i.e., a pair of 
purely imaginary eigenvalues.
Signs of the remaining eigenvalues of $L$ could be judged as follows.

If $D_{a} \geq \frac{l^2+l\sqrt{l^2-4}}{2}$, then $\det(L_k) \geq \det(L_0) > 0$ 
for $k=1,2,\dots$. Moreover, if $m^2<\frac{l^2+l\sqrt{l^2-4}}{2Da}\leq(m+1)^2$,
 $m \in \mathbf{N^{+}}$ and $D_{h}<\bar{r}$, then $\det(L_k) > 0$, $k=1,2,\dots$,
where
\[
\bar{r}=\min_{1\leq k\leq m} \frac{D_{a}k^2\frac{l^2+l\sqrt{l^2-4}}{2}
+\det(J)}{(\frac{l^2+l\sqrt{l^2-4}}{2}-D_{a}k^2)k^2}.
\]
Consequently, the remaining eigenvalues of $L$ all have negative real parts.
If $m^2<$ $\frac{l^2+l\sqrt{l^2-4}}{2Da}\leq (m+1)^2$, 
$m \in \mathbf{N^{+}}$ and $D_{h}>\bar{r}$, then there must exist at least 
one of $\det(L_{1})$, $\det(L_2)$, $\dots$, $\det(L_{m})$ to be negative. 
Then some eigenvalues of $L$ will have positive real parts.

Next the center manifold reduction and normal form technique are applied to 
system \eqref{e1.3}.
Let $Lq = i \omega_0 q$ and $L^{*}q^{*} = -i \omega_0 q^{*}$, then one has 
\[
q =(i \omega_0+ \frac{l^2+l\sqrt{l^2-4}}{2}, -(l^2+l\sqrt{l^2-4}))^{T},
\quad
q^{*} = \frac{1}{2\omega_0}(i, -\frac{\omega_0}{l^2+l\sqrt{l^2-4}}+\frac{i}{2})^{T},
\]
 respectively. Note that
$\langle q^{*}, q \rangle = 1$ and $\langle q^{*}, \bar{q} \rangle = 0$.

According to \cite{Hassard}, for each $U\in Dom(L)$, the pair $(z, w)$ could 
be associated, where
 $U=zq+\bar{z}\bar{q}+w$, $z=\langle q^{*},U\rangle$ and $w=(w_{1},w_2)^{T}$. Then
 \begin{gather*}
 u=(i\omega_0+\frac{l^2+l\sqrt{l^2-4}}{2})z+(-i\omega_0
 +\frac{l^2+l\sqrt{l^2-4}}{2})\bar{z}+w_{1}, \\
 v=-({l^2+l\sqrt{l^2-4}})(z+\bar{z})+w_2.
\end{gather*}
System \eqref{e3.9} in $(z, w)$ coordinates is changed to
\begin{equation} \label{e3.15}
\begin{gathered}
\frac{dz}{dt}=i\omega_0z+\langle q^{*},\widetilde{f} \rangle, \\
 \frac{dw}{dt}=Lw+H(z,\bar{z},w),
\end{gathered}
\end{equation}
where
\begin{gather*}
\widetilde{f}=F(zq+\bar{z}\bar{q}+w,\mu_0),\quad
H(z,\bar{z},w)=\widetilde{f}-\langle q^{*},\widetilde{f}\rangle
q-\langle \bar{q}^{*},\widetilde{f}\rangle \bar{q},
\\
\begin{aligned}
\widetilde{f}&=\frac{1}{2}Q(zq+\bar{z}\bar{q}+w,zq+\bar{z}\bar{q}+w)\\
&\quad +\frac{1}{6}C(zq+\bar{z}\bar{q}+w,zq+\bar{z}\bar{q}+w,zq+\bar{z}\bar{q}+w)
+O(|zq+\bar{z}\bar{q}+w|^{4})\\
&=\frac{1}{2}Q(q,q)z^2+Q(q,\bar{q})z\bar{z}
 +\frac{1}{2}Q(\bar{q},\bar{q})\bar{z}^2
 +O(|z|^{3},|z|\cdot|w|,|w|^2),
\end{aligned}\\
\begin{aligned}
\langle q^{*},\widetilde{f} \rangle
&=\frac{1}{2}\langle q^{*},Q(q,q) \rangle z^2
 +\langle q^{*},Q(q,\bar{q}) \rangle z\bar{z}
 +\frac{1}{2}\langle q^{*},Q(\bar{q},\bar{q})\rangle {z}^2\\
&\quad +O(|z|^{3},|z|\cdot|w|,|w|^2),
\end{aligned}\\
\begin{aligned}
\langle \bar{q}^{*},\widetilde{f} \rangle
&=\frac{1}{2}\langle \bar{q}^{*},Q(q,q) \rangle z^2
 +\langle \bar{q}^{*},Q(q,\bar{q}) \rangle z\bar{z}
 +\frac{1}{2}\langle \bar{q}^{*},Q(\bar{q},\bar{q}) \rangle {z}^2\\
&\quad +O(|z|^{3},|z|\cdot|w|,|w|^2).
\end{aligned}
\end{gather*}
Hence
\[
H(z,\bar{z},w)=\frac{1}{2}z^2H_{20}+z\bar{z}H_{11}
 +\frac{1}{2}\bar{z}^2H_{02}+O(|z|^{3},|z|\cdot|w|,|w|^2),
\]
where
\begin{gather*}
 H_{20}=Q(q,q)-\langle q^{*},Q(q,q) \rangle q-\langle \bar{q}^{*},Q(q,q) \rangle
  \bar{q},\\
 H_{11}=Q(q,\bar{q})-\langle q^{*},Q(q,\bar{q}) \rangle q
 -\langle \bar{q}^{*},Q(q,\bar{q}) \rangle \bar{q},\\
 H_{02}=Q(\bar{q},\bar{q})-\langle q^{*},Q(\bar{q},\bar{q}) \rangle q
 -\langle \bar{q}^{*},Q(\bar{q},\bar{q}) \rangle \bar{q}.
\end{gather*}
Moreover, $H_{20}=H_{11}=H_{02}=(0,0)^{T}$, so
$H(z,\bar{z},w)=O(|z|^{3},|z|\cdot|w|,|w|^2)$.
Hence, system \eqref{e3.9} possesses a center manifold. It can be described as
\[
w=\frac{1}{2}z^2w_{20}+z\bar{z}w_{11}+\frac{1}{2}\bar{z}^2w_{02}+O(|z|^{3}).
\]
In view of $Lw+H(z,\bar{z},w)=\frac{dw}{dt}=\frac{\partial{w}}{\partial{z}}
\frac{dz}{dt}+\frac{\partial{w}}{\partial{\bar{z}}}\frac{d\bar{z}}{dt}$,
one has
\begin{gather*}
 w_{20}=[2i\omega_0-L]^{-1}H_{20}=(0,0)^{T},\\
 w_{11}=-L^{-1}H_{11}=(0,0)^{T},\\
 w_{02}=[-2i\omega_0-L]^{-1}H_{02}=(0,0)^{T}.
\end{gather*}
Thus, the reaction-diffusion system \eqref{e3.9} restricted to the center
 manifold is
\begin{equation} \label{e3.16}
\frac{dz}{dt}=i\omega_0z+\langle q^{*},\widetilde{f} \rangle
=i\omega_0z+\sum_{2\leq i+j \leq3}\frac{g_{ij}}{i!j!}z^{i}\bar{z}^{j}+O(|z|^{4}),
\end{equation}
where
\begin{gather*}
g_{20}=\langle q^{*},Q(q,q)\rangle,\quad
g_{11}=\langle q^{*},Q(q,\bar{q})\rangle, \quad
g_{02}=\langle q^{*},Q(\bar{q},\bar{q})\rangle,\\
g_{21}=2\langle q^{*},Q(w_{11},q)\rangle+\langle q^{*},Q(w_{20},
\bar{q})\rangle+\langle q^{*},C(q,q,\bar{q})\rangle
=\langle q^{*},C(q,q,\bar{q})\rangle.
\end{gather*}
The dynamics of \eqref{e3.9} is determined by that of \eqref{e3.16}.
Furthermore, its Poincar\'{e} normal form could be given in the  form
\begin{equation}
\frac{dz}{dt}=(\alpha(\mu)+i\omega(\mu))z
+z\sum_{j=1}^{M}\delta_{j}(\mu)(z\bar{z})^{j},
\end{equation}
where $z$ is a complex variable, $M\geq1$, and $\delta_{j}(\mu)$ are
complex-valued coefficients. Then one has
\[
\delta_{1}(\mu)
=\frac{g_{20}g_{11}\left[3\alpha(\mu)+i\omega(\mu)\right]}{2\left[\alpha^2(\mu)
+\omega^2(\mu)\right]}
+\frac{|g_{11}|^2}{\alpha(\mu)+i\omega(\mu)}+
\frac{|g_{02}|^2}{2\left[\alpha(\mu)+3i\omega(\mu)\right]}+\frac{g_{21}}{2}.
\]

Note that $\operatorname{Re}(\delta_{1}(\mu_0))
=\operatorname{Re}[\frac{g_{20}g_{11}}{2\omega_0}i+\frac{g_{21}}{2}]$,
 since $\alpha(\mu_0)=0$ and $\omega(\mu_0)=\omega_0>0$.
From 
\begin{gather*}
g_{20}=\frac{1}{\omega_0}\left[(i\omega_0+\mu)^2-4a\mu(i\omega_0+\mu)\right]
\Big(\frac{\omega_0-3i\mu}{2\mu}\Big),\\
g_{11}=\frac{1}{\omega_0}\left[(\mu^2+\omega_0^2)h-4a\mu^2\right]
\Big(\frac{\omega_0-3i\mu}{2\mu}\Big),\\
g_{21}=\frac{1}{\omega_0}(3\mu i-\omega_0)(3\mu^2+\omega_0^2+2i\omega_0\mu),
\end{gather*}
one has
\begin{align*}
\operatorname{Re}(\delta_{1}(\mu_0))=&\frac{1}{4\omega_0^2\mu_0}
\big\{(h_0\mu_0^2+h_0\omega_0^2-4a_0\mu_0^2)[3(h_0\mu_0^2-h_0\omega_0^2
-4a_0\mu_0^2)\\
&-(\omega_0^2-9\mu_0^2)(h_0-2a_0)]-2\omega_0^2\mu_0(\omega_0^2+9\mu_0^2)\big\},
\end{align*}
from which one can obtain that the bifurcated limit cycle is locally stable 
in the center manifold if $\operatorname{Re}(\delta_{1}(\mu_0))<0$, otherwise,
it is unstable in the center manifold. 
In fact, when $\operatorname{Re}(\delta_{1}(\mu_0))<0$, the 
corresponding Floquet exponent is negative, otherwise
the corresponding Floquet exponent is positive.
However, the stability of such homogeneous limit cycle for system \eqref{e1.3} 
may be different for system \eqref{e2.1}. If $P_0$ is unstable for 
system \eqref{e1.3} but stable for system \eqref{e2.1}, 
i.e., some of eigenvalues of system \eqref{e1.3} at the equilibrium point 
$P_0$ have positive real parts, then the limit cycle
bifurcated from Hopf bifurcation will also be unstable for system \eqref{e1.3}. 
That means if some eigenvalue of $L$ has positive real part, then the bifurcated
limit cycle is unstable. When eigenvalues of $L$ have negative real parts 
except a pair of imaginary roots, the limit cycle will be stable 
when $\operatorname{Re}(\delta_{1}(\mu_0))<0$, and unstable when 
$\operatorname{Re}(\delta_{1}(\mu_0))>0$. After tedious calculation, 
it shows that
\[
\operatorname{Re}(\delta_{1}(\mu_0))=\frac{l^2+l\sqrt{l^2-4}}{4\sqrt{l^2-4}}
\Big(5l^3-14l+5l^2\sqrt{l^2-4}+4\sqrt{l^2-4}\Big)>0.
\]
That implies the limit cycle from the Hopf bifurcation is unstable for 
system \eqref{e1.3} under diffusive effects, otherwise, it is stable for
 system \eqref{e2.1}.
Now the above discussions are summarized as in the following theorem.


\begin{theorem} \label{thm3.2}
 Assume \eqref{H2} holds, so the spatially homogeneous periodic solution bifurcated from the equilibrium $P_0(a_0,b_0)$ is stable for system \eqref{e2.1}. However,
 the spatially homogenous periodic solution is always unstable for system \eqref{e1.3} with diffusive terms.
\end{theorem}


\section{Numerical simulations}

In this section, numerical simulations about the Turing and Hopf bifurcation will 
be illustrated. From Theorem \ref{thm3.1}, we know that under conditions \eqref{H1}
and either \eqref{H3} or \eqref{H4}, the point $(a_0, h_0)$ will be still stable, so no Turing instability will be induced. Meanwhile, under \eqref{H1} and \eqref{H5}, the
point $(a_0, h_0)$ will become unstable from stable under diffusive effects, 
so the Turing instability will occur. Consequently,
some patterns will form in the
original system. For further understanding above theoretical analysis, 
the corresponding numerical results are presented.

Now we take parameters as $\mu=1, c=2.2, D_a=1.5, D_h=10$, so \eqref{H1} and 
\eqref{H3} are satisfied. The point $P_0$ is still stable under diffusive effects, see
Figure \ref{fig3}. Initial states are $a(0,t)=1.7179+0.8\cos(x)$, $h(0, t)=0.5821+0.8\cos(x)$.

\begin{figure}[htb]
\centering
 \includegraphics[width=0.48\textwidth]{fig3a} % Fig3a2.eps
 \includegraphics[width=0.48\textwidth]{fig3b} % Fig3h2.eps
\caption{The point $P_0$ is stable.}
\label{fig3}
\end{figure}

If the parameters are taken as $\mu=1, c=2.3, D_a=0.5, D_h=3$, so \eqref{H1}
 and \eqref{H4}  are satisfied. The point $P_0$ is
still stable under diffusive effects, see Figure \ref{fig4}. 
We take $a(0,t)=1.7179+0.5\cos(x)$, $h(0, t)=0.5821+0.5\cos(x)$.

\begin{figure}[ht]
\begin{center}
\includegraphics[width=0.48\textwidth]{fig4a} % Fig4a2.eps
\includegraphics[width=0.48\textwidth]{fig4b} % Fig4h2.eps
\end{center}
\caption{The point $P_0$ is stable.}
\label{fig4}
\end{figure}

However, when $\mu=1$, $c=2.3$, $D_a=0.5$, $D_h=10$, so \eqref{H1} and \eqref{H5}
 are satisfied, the point $P_0$ become unstable under
diffusive effects, see Figure \ref{fig5}. Initial values are taken as 
$a(0,t)=1.7179+0.5\cos(x)$, $h(0, t)=0.5821+0.5\cos(x)$,
Then consequently it is found that the patterns appear, see Figure \ref{fig6}.

\begin{figure}[ht]
\begin{center}
\includegraphics[width=0.48\textwidth]{fig5a} % Fig5a2.eps
\includegraphics[width=0.48\textwidth]{fig5b} % Fig5h2.eps
\end{center}
\caption{The point $P_0$ is unstable with diffusion.}
\label{fig5}
\end{figure}



\begin{figure}[ht]
\begin{center}
\includegraphics[width=0.48\textwidth]{fig6} % Fig5pattern.eps
\end{center}
\caption{Patterns appear in system \eqref{e1.3}.}
\label{fig6}
\end{figure}

From the numerical results, note that the Turing instability of the equilibrium 
point occur under the diffusive effects. As for such effects
on the bifurcated limit cycle, we take $\mu=7.86$, $c=23.58$, $D_a=7.86$, $D_h=5$. 
Then $\mu>\mu_0\approx 7.8541$ and $D_a>\mu_0$, so \eqref{H2} is satisfied and the
eigenvalues of $L$ have negative real parts. In this case, the limit cycle from 
the Hopf bifurcation is stable for system \eqref{e2.1}, but the spatially
homogeneous periodic solution is unstable for system \eqref{e1.3} since 
$\operatorname{Re}(\delta_{1}(\mu_0))>0$, see Figure \ref{fig7}. 
Initial values are taken as
$a(0,t)=2.5+0.5\cos(x)$, $h(0, t)=3+0.5\cos(x)$, close to the limit cycle.


\begin{figure}[ht]
\begin{center}
\includegraphics[width=0.48\textwidth]{fig7a} % Fig7a2.eps
\includegraphics[width=0.48\textwidth]{fig7b} % Fig7h2.eps
\end{center}
\caption{Turing instability of bifurcated periodic solution occurs.}
\label{fig7}
\end{figure}


The similar phenomenon occurs when parameters are taken as 
$\mu=7.86$, $c=23.58$, $D_a=7$, $D_h=2$, then $\mu>\mu_0\approx 7.8541$,
$D_a<\mu_0$ and $D_h<\bar{r}$, so \eqref{H2} is satisfied and the
eigenvalues of $L$ have negative real parts. In this case, the limit cycle 
from the Hopf bifurcation is stable for system \eqref{e2.1},
but the spatially homogeneous periodic solution is unstable for 
system \eqref{e1.3}, see Figure \ref{fig8}. Initial values are taken as
$a(0,t)=2+0.02\operatorname{rand}(1)$, $h(0, t)=3+0.02\operatorname{rand}(1)$, 
close to the limit cycle.

\begin{figure}[ht]
\begin{center}
 \includegraphics[width=0.48\textwidth]{fig8a} % Fig8a2.eps
 \includegraphics[width=0.48\textwidth]{fig8b} % Fig8h2.eps
\end{center}
\caption{Turing instability of bifurcated periodic solution occurs.}
\label{fig8}
\end{figure}

\begin{figure}[ht] 
\begin{center}
 \includegraphics[width=0.48\textwidth]{fig9a} % Fig9a2.eps
 \includegraphics[width=0.48\textwidth]{fig9b} % Fig9h2.eps
\end{center}
\caption{Turing instability of bifurcated periodic solution occurs under diffusion.}
\label{fig9}
\end{figure}

Further, the Turing instability still occur when parameters are taken as 
$\mu=7.86$, $c=23.58$, $D_a=2$, $D_h=10.6$,
then $\mu>\mu_0\approx 7.8541$, $D_a<\mu_0$ and $D_h>\bar{r}$, so \eqref{H2} 
is satisfied and some eigenvalues of $L$ have positive real parts.
 The limit cycle from the Hopf bifurcation is still stable for system \eqref{e2.1}, 
but it is unstable for system \eqref{e1.3}, see Figure \ref{fig9}. Initial
 values are taken as $a(0,t)=2.6+0.5\operatorname{rand}(1)$, 
$h(0, t)=3.1+0.5 \operatorname{rand}(1)$, close to the limit cycle.

From the numerical simulations in Figures \ref{fig7}--\ref{fig9}, 
it shows that some patterns like stripe and spike solutions appear in 
system \eqref{e1.3}.
Figure \ref{fig10} corresponds to the cases in Figures \ref{fig7} and \ref{fig8}.
 Figure \ref{fig11} is the pattern in Figure \ref{fig9}.

\begin{figure}[ht] 
\begin{center}
 \includegraphics[width=0.48\textwidth]{fig10} % Fig8pattern.eps
\end{center}
\caption{Patterns appearing in system \eqref{e1.3}.}
\label{fig10}
\end{figure}

\begin{figure}[ht!] 
\begin{center}
 \includegraphics[width=0.48\textwidth]{fig11} % Fig9pattern.eps
\end{center}
\caption{Patterns appearing in system \eqref{e1.3}.}
\label{fig11}
\end{figure}

\subsection*{Conclusions}
To understand the dynamical behavior under diffusive effects, 
we consider the Gierer-Meinhardt depletion model here. The model is commonly used to
explain the underlying complex mechanism for pattern formation in nature, 
describing the interaction of two sources in processes such as biological and 
chemical ones. If the equilibrium points and periodic solutions become unstable 
under diffusion terms, it is said to be the Turing instability, namely,
the diffusion-driven instability. It is frequently noted that on such occasions 
some patterns will form in the system. By dynamical techniques,
stability and the Hopf bifurcation of fixed points are analyzed in detail. 
Afterwards, it shows that the Turing instability will occur under some
conditions, with the diffusive effects on stable fixed points and the stable 
bifurcated limit cycle. That implies the spatially nonhomogeneous
solutions will appear in the system, which will cause the formation of patterns. 
Numerical simulations verify the effectiveness of theoretical
analysis. The other complex and interesting dynamical behaviors related to such 
model will be further investigated.


\subsection*{Acknowledgments}
This work was supported by the National Science Foundation of China 
(No. 11571016, 61403115), and by the Specialized Research Fund for the
Doctoral Program of Higher Education of China (No. 20093401120001).

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\end{document}


