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\AtBeginDocument{{\noindent\small
\emph{Electronic Journal of Differential Equations},
Vol. 2014 (2014), No. 188, pp. 1--28.\newline
ISSN: 1072-6691. URL: http://ejde.math.txstate.edu or http://ejde.math.unt.edu
\newline ftp ejde.math.txstate.edu}
\thanks{\copyright 2014 Texas State University - San Marcos.}
\vspace{9mm}}

\begin{document}
\title[\hfilneg EJDE-2014/188\hfil Chaotic oscillations]
{Chaotic oscillations of the Klein-Gordon equation with
distributed energy pumping and van der Pol boundary regulation and
distributed time-varying coefficients}

\author[B. Sun, T. Huang \hfil EJDE-2014/188\hfilneg]
{Bo Sun, Tingwen Huang}  % in alphabetical order

\address{Bo Sun \newline
Department of Mathematics, Changsha University of Science and Technology,
Changsha, Hunan, China}
\email{sunbo1965@yeah.net}

\address{Tingwen Huang \newline
Science Program, Texas A\&M University at Qatar,
Education City, Doha, Qatar}
\email{tingwen.huang@qatar.tamu.edu}

\thanks{Submitted August 1, 2014. Published September 10, 2014.}
\subjclass[2000]{35L05, 35L70, 58F39, 70L05}
\keywords{Chaotic Oscillations; Klein-Gordon equation; \hfill\break\indent
distributed energy pumping; van der Pol boundary regulation}

\begin{abstract}
 Consider the Klein-Gordon equation with variable coefficients, a
 van der Pol cubic nonlinearity in one of the boundary conditions and
 a spatially distributed \emph{antidamping} term, we use a
 \emph{variable-substitution} technique together with the analogy with
 the 1-dimensional wave equation to prove that for the Klein-Gordon
 equation chaos occurs for a class of equations and boundary
 conditions when system parameters enter a certain regime. Chaotic
 and nonchaotic profiles of solutions are illustrated by computer
 graphics.
\end{abstract}

\maketitle
\numberwithin{equation}{section}
\numberwithin{figure}{section}
\newtheorem{theorem}{Theorem}[section]
\newtheorem{lemma}[theorem]{Lemma}
\newtheorem{remark}[theorem]{Remark}
\newtheorem{example}[theorem]{Example}
\allowdisplaybreaks

\section{Introduction}

 During the past decade, progress has been made in dynamical system
theory in proving the onset of chaos in the 1D wave equation and the
Klein-Gordon equation with a van der Pol cubic nonlinearity in one
of the boundary conditions and a spatially distributed
\emph{antidamping} term, see
\cite{ChHs1,ChHs2,ChHs3,ChHs4,ChHs5,ChSb}. The basic method is 
\emph{characteristic reflections}, by which discrete dynamical systems are
extracted. We first give a quick review of the work mentioned above,
where the main motivating interest was the significance in 
\emph{nonlinear feedback boundary control}. For the wave equation
\begin{equation}\label{KGeq1.1}
w_{tt}(x,t)-c^2w_{xx}(x,t) = 0,\quad 0<x<1,\; t>0,\; c>0,
\end{equation}
we assume that at the left-end $x=0$, the boundary condition is
\begin{equation}\label{KGeq1.2}
w_t(0,t) = -\eta w_x(0,t),\quad t>0,\; \eta>0,\; \eta\ne c,
\end{equation}
and at the right-end $x=1$, the boundary condition is of the van der
Pol type:
\begin{equation}\label{KGeq1.3}
w_x(1,t) = \alpha w_t(1,t) - \beta w^3_t(1,t),\quad t>0,\;
0<\alpha<c,\; \beta>0.
\end{equation}
Then the energy functional
\begin{equation}\label{KGeq1.4}
E(t) = \frac12 \int^1_0 \Big[w^2_x(x,t)  + \frac1{c^2}w^2_t(x,t)\Big] dx
\end{equation}
\emph{rises} if $|w_t(1,t)|$ is small, and \emph{falls} if
$|w_t(1,t)|$ is large. Thus, the van der Pol boundary condition
\eqref{KGeq1.3} has a \emph{self-regulating effect}. This can cause
chaos to occur in $w_x$ and $w_t$ if the parameters $\alpha,c$ and
$\eta$ enter a certain regime.

The treatment in \cite{ChHs3} relies heavily on the \emph{method of
characteristics} for linear hyperbolic systems and simple
wave-reflecting relations. Let $c=1$, and
\begin{equation}
u(x,t)=\frac{1}{2}[w_x(x,t)+w_t(x,t)],\quad
v(x,t)=\frac{1}{2}[w_x(x,t)-w_t(x,t)].
\end{equation}
Then
\begin{gather}
v(0,t)=G_{\eta}(u(0,t))\equiv \frac{1+\eta}{1-\eta}u(0,t), \\
u(1,t)=F_{\alpha,\beta}(v(1,t)),
\end{gather}
where $F_{\alpha,\beta}:\mathbb{R}\rightarrow\mathbb{R}$ is a
nonlinear mapping such that for each given $v\in\mathbb{R}$, 
$u= F_{\alpha,\beta}(v)$ is the unique solution of the cubic equation
\begin{equation}
\beta (u-v)^3+(1-\alpha)(u-v)+2v=0.
\end{equation}
Therefore, $u(x,t)$ and $v(x,t)$ for $x\in [0,1]$ and 
$t\in (0,\infty)$ are determined by the initial data $u(x,0)$, $v(x,0)$
and the iterative composition of $F_{\alpha,\beta}\circ G_{\eta}$ or
$G_{\eta}\circ F_{\alpha,\beta}$. Finally, the chaotic dynamics in
the 1D wave equation is reduced to the discrete dynamical system
generated by the interval map $F_{\alpha,\beta}\circ G_{\eta}$ or
$G_{\eta}\circ F_{\alpha,\beta}$.

A generalization of the 1D wave equation is the Klein-Gordon
equation described as
\begin{equation}\label{KGeq1.5}
w_{tt}(x,t) + \eta w_t(x,t) - w_{xx}(x,t) + k^2w(x,t) = 0,\quad
0<x<1,\; t>0,
\end{equation}
where $k\neq 0$, $\eta>0$. A special case is
\begin{equation}\label{KGeq1.6}
w_{tt}+2kw_t - w_{xx} + k^2w=0, \quad \text{for } (x,t)\in
(0,1)\times (0,\infty).
\end{equation}

We consider, for \eqref{KGeq1.6}, the following boundary condition,
\begin{gather}\label{KGeq1.7}
w_t(0,t) + kw(0,t) = -\lambda w_x(0,t),\quad t>0, 
 \text{ at $x=0$,  for given } \lambda\in \mathbb{R};\\
\label{KGeq2.26}
w_x(1,t) = \alpha[w_t(1,t)+kw(1,t)] - \beta[w_t(1,t)+kw(1,t)]^3,\quad t>0, 
\text{ at } x=1,
\end{gather}
where $0<\alpha<1$, $\beta>0$;
and the energy function
\begin{equation}\label{KGeq1.8}
\widetilde E(t) = \frac12 \int^1_0 [w^2_x+(w_t+kw)^2]dx.
\end{equation}
Then $\frac{d}{dt}\widetilde E(t)$ is indefinite, which is the sign
of chaos.

The simple change of variable
\begin{equation}
w(x,t) = e^{-kt}W(x,t)
\end{equation}
leads to
\begin{equation}
\frac{\partial^2}{\partial x^2} W(x,t) - \frac{\partial^2}{\partial
t^2} W(x,t) = 0.
\end{equation}
Define
\begin{equation}\label{KGeq1.9}
u=\frac12(w_x+w_t+kw), \quad v=\frac12(w_x-w_t-kw).
\end{equation}
Then
\begin{equation}\label{KGeq1.10}
v(0,t) = \frac{1+\lambda}{1-\lambda} u(0,t)\equiv G_\lambda(u(0,t)),
\end{equation}
where $G_\lambda$ is defined to be the linear operator of
multiplication by $(1+\lambda)/(1-\lambda)$. Also we have
\begin{equation}\label{KGeq1.11}
\beta[u(1,t)-v(1,t)]^3 + (1-\alpha) [u(1,t)-v(1,t)] + 2v(1,t) = 0.
\end{equation}

For any $v\in {\mathbb{R}}$, define $g(v)$ to be the \emph{unique real}
solution to the cubic equation
\begin{equation}\label{KGeq1.12}
\beta g(v)^3 + (1-\alpha) g(v)+2v=0,
\end{equation}
 and
\begin{equation}\label{KGeq1.13}
F(v) \equiv F_{\alpha,\beta}(v) \equiv v+g_{\alpha,\beta}(v).
\end{equation}
Then for each given $v(1,t)$, equation \eqref{KGeq1.11} has a unique
solution $u(1,t)$ given by
\[
u(1,t) = F_{\alpha,\beta}(v(1,t)).
\]

It is easy to check that $e^{kt}u(x,t)$ keeps constant along each
characteristics $x+t=c$, and $e^{kt}v(x,t)$ keeps constant along
each characteristics $x-t=c$. Therefore, we have
\begin{equation}\label{KGeq1.14}
\begin{gathered}
      u(1,t+2) = F_{\alpha,\beta}(G_\lambda(e^{-2k}u(1,t))),\\
v(0,t+2) = G_\lambda(e^{-k}F_{\alpha,\beta}(e^{-k}v(0,t))),
      \end{gathered}
\end{equation}
for any $t>0$. Finally, the dynamics of
\begin{equation}
u=\frac12(w_x+w_t+kw), \quad v=\frac12(w_x-w_t-kw)
\end{equation}
are determined by the iterative compositions of the functions
$F_{\alpha,\beta}(G_\lambda(e^{-2k}\cdot))$ or
$G_\lambda(e^{-k}F_{\alpha,\beta}(e^{-k}\cdot))$.

One can imagine that there may be more chaos in the Klein-Gordon
equation if its constant coefficients are replaced by variable
coefficients. So in this paper we consider more general situations
and problems below:
\begin{equation}\label{KGeq1.15}
[\frac{\partial}{\partial t}-a(x)\frac{\partial}{\partial x}+k_1]
[\frac{\partial}{\partial t}+b(x)\frac{\partial}{\partial
x}+k_2]w(x,t)=0, \quad \text{for} \quad x\in (0,1), \quad t>0
\end{equation}
with some linear and cubic nonlinear boundary condition, where
 $a(x)>0$ and $b(x)>0$ are continuous real functions defined
on $[0,1]$.

The organization of this article is  as follows:
In Section 2, we consider a simple case with $a(x)\equiv Kb(x)$,
and $k_1=k_2=0$, where $K$ is a positive constant.
In Section 3, we consider some more cases with $a(x)\equiv Kb(x)$, 
and $k_1$, $k_2\in \mathbb{R}$.
In Section 4, we prove the bifurcation from a stable fixed point to chaos.
In Section 5, we consider some more general cases.

\section{Klein-Gordon Equation with variable coefficients
but no state term}

Let us consider a simple case of \eqref{KGeq1.15} with $k_1=k_2=0$;
i.e.,
\begin{equation}\label{2.1}
[\frac{\partial}{\partial t}-a(x)\frac{\partial}{\partial x}]
[\frac{\partial}{\partial t}+b(x)\frac{\partial}{\partial x}]w=0,
\quad \text{for } x\in (0,1),\; t>0.
\end{equation}
Let
\begin{equation}\label{variableSubstitution}
\xi=\int_0^x\frac{dx}{a(x)}, \quad \eta=\int_0^x\frac{dx}{b(x)},
\end{equation}
then it follows from $a=Kb$ that $\eta =K\xi$, and thus
\begin{equation*}
\frac{\partial}{\partial \xi}=K\frac{\partial}{\partial \eta}.
\end{equation*}

Let $\tilde{w}(\eta,t)=w(x,t)$, then \eqref{2.1} is equivalent to
\begin{equation}
[\frac{\partial}{\partial t}-K\frac{\partial}{\partial \eta}]
[\frac{\partial}{\partial t}+\frac{\partial}{\partial \eta}]\tilde{w}=0,
\end{equation}
or
\begin{equation}
[\frac{\partial}{\partial t}+\frac{\partial}{\partial \eta}]
[\frac{\partial}{\partial t}-K\frac{\partial}{\partial \eta}]\tilde{w}=0.
\end{equation}
It follows immediately that
\begin{gather*}
\tilde{w}_{\eta}+\tilde{w}_t=f(\eta +Kt),\\
K\tilde{w}_{\eta}-\tilde{w}_t=g(t-\eta)
\end{gather*}
for some functions $f$ and $g$ depending on the initial data.
Let
\begin{gather*}
\tilde{u}(\eta,t)=\frac{1}{2}[\tilde{w}_{\eta}+\tilde{w}_t],\\
\tilde{v}(\eta,t)=\frac{1}{2}[K\tilde{w}_{\eta}-\tilde{w}_t].
\end{gather*}
Then $\tilde{u}$ keeps constant along lines $\eta +Kt=c$, and $\tilde{v}$ 
keeps constant along lines $\eta-t=c$.

We impose nonlinear boundary conditions as
\begin{gather}
\tilde{w}_t(0,t)=-\lambda \tilde{w}_{\eta}(0,t),\label{zuobianjie} \\
 \tilde{w}_{\eta}(L,t)=\alpha \tilde{w}_t(L,t)
 -\beta \tilde{w}_t^3(L,t),\label{youbianjie}
\end{gather}
where $L=\int_0^1\frac{dx}{b(x)}$.
Then
\begin{gather}
\tilde{v}(0,t)=G_{K,\lambda}(\tilde{u}(0,t))
=\frac{K+\lambda}{1-\lambda}\tilde{u}(0,t),\\
\tilde{u}(L,t)=F_{K,\alpha,\beta}(\tilde{v}(L,t)),
\end{gather}
where $u=F_{K,\alpha,\beta}(v)$ is the unique real solution of the cubic equation
\begin{align}\label{cubicEquation}
\frac{4\beta}{(K+1)^2}(Ku-v)^3+(\frac{1}{K}-\alpha )(Ku-v)+(\frac{1}{K}+1)v=0.
\end{align}
It follows from \eqref{variableSubstitution} that
\begin{equation}
 d\xi=\frac{dx}{a(x)}, \quad d\eta=\frac{dx}{b(x)},
\end{equation}
and thus
\begin{gather}
\frac{\partial w}{\partial x} =\frac{\partial \tilde{w}}{\partial
\xi}\frac{d\xi}{dx}=\frac{1}{a(x)}\frac{\partial \tilde{w}}{\partial \xi},
\\
\frac{\partial w}{\partial x} =\frac{1}{b(x)}\frac{\partial
\tilde{w}}{\partial \eta},
\end{gather}
or
\begin{gather}
\frac{\partial \tilde{w}}{\partial \xi}=a(x)\frac{\partial
w}{\partial x}, \\
\frac{\partial \tilde{w}}{\partial \eta}=b(x)\frac{\partial
w}{\partial x}.
\end{gather}
 So the boundary condition \eqref{zuobianjie}-\eqref{youbianjie} is equivalent to
\begin{gather}
w_t(0,t)=-\lambda b(0)w_x(0,t), \label{2.1leftBoundary}\\
 b(1)w_x(1,t)=\alpha w_t(1,t)-\beta w_t^3(1,t). \label{2.1rightBoundary}
\end{gather}
Let
\begin{gather*}
 u(x,t)=\tilde{u}(\eta,t)=\frac{1}{2}[b(x)w_x+w_t], \\
v(x,t)=\tilde{v}(\eta,t)=\frac{1}{2}[a(x)w_x-w_t],
\end{gather*}
then
\begin{gather}
v(0,t)=G_{K,\lambda}(u(0,t))=\frac{K+\lambda}{1-\lambda}u(0,t),\\
u(1,t)=F_{K,\alpha,\beta}(v(1,t)).
\end{gather}
Therefore
\begin{gather}
u(1,t)=F_{K,\alpha,\beta}(G_{K,\lambda}(u(1,t-L-\frac{L}{K})),\label{reflection2.1} \\
v(0,t)=G_{K,\lambda}(F_{K,\alpha,\beta}(v(0,t-L-\frac{L}{K})).\label{reflection2.2}
\end{gather}

The dynamics of $u$ and $v$ are reduced to the properties of $G\circ F$ 
and $F\circ G$.
Define a function $\psi(x)=\int_0^x\frac{dx}{b(x)}$ on $[0,1]$, 
then $\psi$ is one to one.

\begin{lemma}[Solution representations for $u(x,t)$ and $v(x,t)$]\label{Lemma2.1}
Assume \eqref{2.1}, \\ \eqref{2.1leftBoundary} and \eqref{2.1rightBoundary}. 
Then for any $x$: $0<x<1$, and $t>0$, we have, for $t$: 
$t=(1+\frac{1}{K})jL+\tau$, $j=0,1,2,\dots$, $\tau >0$,
\begin{gather*}
u(x,t) =\begin{cases}
(F_{\alpha,\beta}\circ G_{\lambda,K})^j (F_{\alpha,\beta}
(v_0(\psi^{-1}(1+\frac{1}{K})L-\tau-\frac{\eta}{K}))), \\
\quad \text{if } L\le K\tau +\eta \le (K+1)L;\\[4pt]
(F_{\alpha,\beta}\circ G_{\lambda,K})^{j+1}(u_0(\psi^{-1}(K\tau+\eta-(K+1)L)))),\\
\quad \text{if } (K+1)L \le K\tau +\eta \le (K+2)L;
\end{cases}
\\[4pt]
v(x,t) =\begin{cases}
(G_{\lambda,K}\circ F_{\alpha,\beta}))^j (G(u_0(\psi^{-1}(K(\tau-\eta))))),\\
\quad \text{if }  t=(1+\frac{1}{K})jL+\tau, \quad 0\le \tau -\eta \le \frac{L}{K};
\\[4pt]
(G_{\lambda,K}\circ F_{\alpha,\beta}))^{j+1}
(v_0(\psi^{-1}(1+\frac{1}{K})L-\tau+\eta)), \\
\quad \text{if }  \frac{L}{K} \le \tau -\eta \le (1+\frac{1}{K})L.
\end{cases}
\end{gather*}
\end{lemma}



\begin{lemma}[Derivative Formulas]\label{Lemma2.2}
Let  $0<\alpha\le \frac{1}{K}$, $\beta >0$ and $\eta >0$, $\eta \neq 1$, 
where $\alpha$ and $\beta$ are given and fixed, but $\eta$ is a varying parameter. 
Define
\[
f_1(v,\eta)=G\circ F(v)=\frac{K+\eta}{1-\eta}F(v),\quad 
f_2(v,\eta)=F\circ G(v)=F(\frac{K+\eta}{1-\eta}v),\quad v\in \mathbb{R}.
\]
Let $g(v)$ be the unique real solution of the cubic equation
\begin{equation}\label{g}
\frac{4\beta}{(K+1)^2}g(v)^3+(\frac{1}{K}-\alpha)g(v)+(\frac{1}{K}+1)v=0,
\end{equation}
for a given $v\in \mathbb{R}$.
Then
\begin{gather}
\frac{\partial}{\partial v}f_1(v,\eta)
=\frac{K+\eta}{K(1-\eta)}[1-\frac{K+1}
{\frac{12K\beta}{(K+1)^2}g(v)^2+1-K\alpha}],\label{Derivative1}
\\
\frac{\partial}{\partial v}f_2(v,\eta)
=\frac{K+\eta}{K(1-\eta)}[1-\frac{K+1}{\frac{12K\beta}{(K+1)^2}
g(\frac{K+\eta}{1-\eta}v)^2+1-K\alpha}], 
\notag \\
\frac{\partial}{\partial \eta}f_1(v,\eta)
=\frac{1+K}{K(1-\eta)^2}[v+g(v)],
\notag \\
\frac{\partial}{\partial \eta}f_2(v,\eta)
=\frac{1+K}{K(1-\eta)^2}[1-\frac{K+1}{\frac{12K\beta}{(K+1)^2}
g(\frac{K+\eta}{1-\eta}v)^2+1-K\alpha}]v,
\notag \\
\frac{\partial^2}{\partial \eta \partial v}f_1(v,\eta)
=\frac{K+1}{K(1-\eta)^2}
[1-\frac{K+1}{\frac{12K\beta}{(K+1)^2}g(v)^2+1-K\alpha}],
\notag \\
\frac{\partial^2}{\partial v^2}f_1(v,\eta)
=\frac{K+\eta}{(1-\eta)}(-24)\beta\cdot \frac{g(v)}{[\frac{12K\beta}{(K+1)^2}
g(v)^2+1-K\alpha]^3},
\notag \\
\frac{\partial^3}{\partial v^3}f_1(v,\eta)
=\frac{K+\eta}{1-\eta}24(K+1)\beta\frac{ 1-K\alpha -\frac{60K\beta}{(K+1)^2}
g(v)^2}{[\frac{12K\beta}{(K+1)^2}g(v)^2+1-K\alpha]^5}.
\end{gather}
\end{lemma}

\begin{lemma}
[Intersections with the Lines $u-v=0$ and $u+v=0$]\label{Lemma2.3}
Let  $0<\alpha\le 1/K$, $\beta >0$, $\eta >0$,
$\eta \neq 1$ be given. Then

{\rm (i)} $u=G\circ F(v)$ intersects the line $u=v$ at the points
\begin{align*}
(u,v)&=(-\frac{K+\eta}{2\eta}\sqrt{\frac{1+\alpha\eta}{\beta\eta}}, 
   -\frac{K+\eta}{2\eta}\sqrt{\frac{1+\alpha\eta}{\beta\eta}}), \\
&\quad (0,0), \\
&\quad  (\frac{K+\eta}{2\eta}\sqrt{\frac{1+\alpha\eta}{\beta\eta}},
   \frac{K+\eta}{2\eta}\sqrt{\frac{1+\alpha\eta}{\beta\eta}});
\end{align*}

{\rm (ii)} $u=G\circ F(v)$ intersects the line $u=-v$ at the points
\begin{align*}
 (u,v)&=(-\frac{(K+1)(K+\eta)}{2[2K+(1-K)\eta]}
\sqrt{\frac{(1 +2\alpha )K-1 +[2+\alpha(1-K)]\eta}{[2K+(1-K)\eta]\beta}},\\
&\quad  \frac{(K+1)(K+\eta)}{2[2K+(1-K)\eta]}\sqrt{\frac{(1 +2\alpha )K-1 
+[2+\alpha(1-K)]\eta}{[2K+(1-K)\eta]\beta}}), \\
&\quad (0,0), \\
&\quad 
 (\frac{(K+1)(K+\eta)}{2[2K+(1-K)\eta]}\sqrt{\frac{(1 +2\alpha )K-1 
+[2+\alpha(1-K)]\eta}{[2K+(1-K)\eta]\beta}},\\
&\quad -\frac{(K+1)(K+\eta)}{2[2K+(1-K)\eta]}\sqrt{\frac{(1 +2\alpha )K-1 
+[2+\alpha(1-K)]\eta}{[2K+(1-K)\eta]\beta}});
\end{align*}

{\rm (iii)} $u=F\circ G(v)$ intersects the line $u=v$ at the points
\begin{align*}
(u,v)&=(-\frac{1-\eta}{2\eta}\sqrt{\frac{1+\alpha\eta}{\beta\eta}},
 -\frac{1-\eta}{2\eta}\sqrt{\frac{1+\alpha\eta}{\beta\eta}}), \\\
&\quad(0,0), \\
&\quad (\frac{1-\eta}{2\eta}\sqrt{\frac{1+\alpha\eta}{\beta\eta}},
\frac{1-\eta}{2\eta}\sqrt{\frac{1+\alpha\eta}   {\beta\eta}});
\end{align*}

{\rm (iv)} $u=F\circ G(v)$ intersects the line $u=-v$ at the points
\begin{align*}
(u,v)&=(-\frac{(1-\eta)(K+1)}{2[2K+ (1-K)\eta]}\sqrt{\frac{(1+2\alpha)
K-1+[2+\alpha (1-K)]\eta}{\beta [2K+(1-K)\eta]}}, \\
&\quad \frac{(1-\eta)(K+1)}{2[2K+ (1-K)\eta]}
\sqrt{\frac{(1+2\alpha)K-1+[2+\alpha (1-K)]\eta}{\beta [2K+(1-K)\eta]}}), \\
&\quad (0,0), \\
&\quad (\frac{(1-\eta)(K+1)}{2[2K+ (1-K)\eta]}
   \sqrt{\frac{(1+2\alpha)K-1+[2+\alpha (1-K)]\eta}{\beta [2K+(1-K)\eta]}},\\
&\quad  -\frac{(1-\eta)(K+1)}{2[2K+ (1-K)\eta]}
   \sqrt{\frac{(1+2\alpha)K-1+[2+\alpha (1-K)]\eta}{\beta [2K+(1-K)\eta]}}).
\end{align*}
\end{lemma}

\begin{remark} \label{rmk2.4} \rm
Conclusions (ii) and (iv) are based on the assumption that
\begin{equation}
\frac{(1+2\alpha)K-1+[2+\alpha (1-K)]\eta}{\beta [2K+(1-K)\eta]}
\geq 0.
\end{equation}
So we assume $K\le 1$ and $(1+2\alpha)K\geq 1$ for conclusions (ii)
and (iv). We also make this assumption for some related results
below, e.g., (ii) and (iv) in Lemma \ref{boundedInvariantSet}.
\end{remark}

\begin{lemma}[$v$-axis Intercepts]\label{lem2.4}
Let  $0<\alpha\le \frac{1}{K}$, $\beta >0$, $\eta >0$, $\eta \neq 1$ 
be given. Then

{\rm (i)} $u=G\circ F(v)$ has $v$-axis intercepts
$v=-\frac{K+1}{2}\sqrt{\frac{1+\alpha}{\beta}}$, $0$, 
$\frac{K+1}{2}\sqrt{\frac{1+\alpha}{\beta}}$;

{\rm (ii)} $u=F\circ G(v)$ has $v$-axis intercepts
\[
v=-\frac{(K+1)(1-\eta)}{2(K+\eta)}\sqrt{\frac{1+\alpha}{\beta}}, \quad
0, \quad 
\frac{(K+1)(1-\eta)}{2(K+\eta)}\sqrt{\frac{1+\alpha}{\beta}}.
\]
 \end{lemma}

\begin{lemma}[Local Maximum, Minimum and Piecewise Monotonicity]
Let $0<\alpha\le \frac{1}{K}$, $\beta >0$, $\eta >0$, $\eta \neq 1$
 be given. Then

{\rm (i)} If $0<\eta<1$, then $G\circ F$ has local extremal values
\begin{gather*}
 M=G\circ F(-v_c)=\frac{K+\eta}{1-\eta}\frac{1+\alpha}{3}
 \sqrt{\frac{1+\alpha}{3\beta}}, \\
 m=G\circ F(v_c)=-\frac{K+\eta}{1-\eta}\frac{1+\alpha}{3}
 \sqrt{\frac{1+\alpha}{3\beta}},
\end{gather*}
   where $v_c=\frac{3+(1-2\alpha)K}{6}\sqrt{\frac{1+\alpha}{3\beta}}$, and 
$M$, $m$ are, respectively, the local
   maximum and minimum of $G\circ F$. The function $G\circ F$ is strictly 
increasing on $(-\infty, -v_c)$ and $(v_c, \infty)$, but strictly decreasing 
on $(-v_c, v_c)$.

   On the other hand, if $\eta>1$, then $G\circ F$ has local minimum ($m$) 
and maximum ($M$) values
\begin{gather*}
m=G\circ F(-v_c)=\frac{K+\eta}{1-\eta}\frac{1+\alpha}{3}
\sqrt{\frac{1+\alpha}{3\beta}}, \\
M=G\circ F(v_c)=-\frac{K+\eta}{1-\eta}\frac{1+\alpha}{3}
\sqrt{\frac{1+\alpha}{3\beta}},
\end{gather*}
   where $v_c$ is the same as above. The function $G\circ F$ is strictly 
decreasing on $(-\infty, -v_c)$ and
   $(v_c,\infty)$, but strictly increasing on $(-v_c,v_c)$.

{\rm (ii)} If $0<\eta<1$, then $F\circ G$ has local extremal values
\begin{gather*}
M=F\circ G(-\tilde{v}_c)=\frac{1+\alpha}{3}\sqrt{\frac{1+\alpha}{3\beta}}, \\
m=F\circ G(\tilde{v}_c)=-\frac{1+\alpha}{3}\sqrt{\frac{1+\alpha}{3\beta}},
\end{gather*}
where $\tilde{v}_c=\frac{1-\eta}{K+\eta}\frac{3+(1-2\alpha)K}{6}
\sqrt{\frac{1+\alpha}{3\beta}}$, and $M$, $m$ are, respectively, the local
maximum and minimum of $F\circ G$. The function $F\circ G$ is strictly 
increasing on $(-\infty, -\tilde{v}_c)$ and $(\tilde{v}_c, \infty)$, 
but strictly decreasing on $(-\tilde{v}_c, \tilde{v}_c)$.

   On the other hand, if $\eta>1$, then $F\circ G$ has local extremal values
\begin{gather*}
m=F\circ G(-\tilde{v}_c)=-\frac{1+\alpha}{3}\sqrt{\frac{1+\alpha}{3\beta}},\\
M=F\circ G(\tilde{v}_c)=\frac{1+\alpha}{3}\sqrt{\frac{1+\alpha}{3\beta}}.
\end{gather*}
 The function $F\circ G$ is strictly decreasing on $(-\infty, -\tilde{v}_c)$ 
and $(\tilde{v}_c, \infty)$, but strictly increasing on 
$(-\tilde{v}_c, \tilde{v}_c)$.
\end{lemma}

\begin{lemma}[Bounded Invariant Intervals]\label{boundedInvariantSet}
Let  $0<\alpha\le \frac{1}{K}$, $\beta >0$, $\eta >0$, $\eta \neq 1$.

{\rm (i)} If $0<\eta<1$ and
\[
M=\frac{K+\eta}{1-\eta}\frac{1+\alpha}{3}\sqrt{\frac{1+\alpha}{3\beta}}
\le\frac{K+\eta}{2\eta}\sqrt{\frac{1+\alpha\eta}{\beta\eta}},
\]
then the iterates of every point in the set 
\[
U\equiv (-\infty,-\frac{K+\eta}{2\eta}\sqrt{\frac{1+\alpha\eta}{\beta\eta}})
\cup (\frac{K+\eta}{2\eta}\sqrt{\frac{1+\alpha\eta}{\beta\eta}},\infty)
\] 
escape to $\pm \infty$,
while those of any point in $\mathbb{R}\backslash\bar{U}$ are attracted to the 
bounded invariant interval
$\mathcal{I}\equiv [-M,M]$ of $G\circ F$.

{\rm (ii)} If $\eta >1$ and
\begin{align*}
M&=-\frac{K+\eta}{1-\eta}\frac{1+\alpha}{3}\sqrt{\frac{1+\alpha}{3\beta}}\\
&\le \frac{(K+1)(K+\eta)}{2[2K+(1-K)\eta]}\sqrt{\frac{(1 +2\alpha)K-1
+[2+\alpha(1-K)]\eta}{[2K+(1-K)\eta]\beta}},
\end{align*}
 then the same conclusion as in (i) holds, with
\begin{align*}
U&\equiv (-\infty, -\frac{(K+1)(K+\eta)}{2[2K+(1-K)\eta]}\sqrt{\frac{(1 +2\alpha)K-1
+[2+\alpha(1-K)]\eta}{[2K+(1-K)\eta]\beta}})\\
&\cup (\frac{(K+1)(K+\eta)}{2[2K+(1-K)\eta]}\sqrt{\frac{(1 +2\alpha)K-1
+[2+\alpha(1-K)]\eta}{[2K+(1-K)\eta]\beta}},\infty)
\end{align*}
and  ${\mathcal{I}}\equiv [-M,M]$ for $G \circ F$.

{\rm (iii)} If $0<\eta<1$ and
$M=\frac{1+\alpha}{3}\sqrt{\frac{1+\alpha}{3\beta}} 
\le \frac{1-\eta}{2\eta}\sqrt{\frac{1+\alpha\eta}{\beta\eta}}$,
 then the same conclusion holds, with
\[
 U\equiv (-\infty, -\frac{1-\eta}{2\eta}\sqrt{\frac{1+\alpha\eta}{\beta\eta}})\cup
 (\frac{1-\eta}{2\eta}\sqrt{\frac{1+\alpha\eta}{\beta\eta}},\infty)
\]
 and ${\mathcal{I}}=[-M,M]$ for $F\circ G$.

{\rm (iv)} If $\eta>1$ and
\[
 M=\frac{1+\alpha}{3}\sqrt{\frac{1+\alpha}{3\beta}}\le
-\frac{(1-\eta)(K+1)}{2[2K+ (1-K)\eta]}
\sqrt{\frac{(1+2\alpha)K-1+[2+\alpha (1-K)]\eta}{\beta
[2K+(1-K)\eta]}}),
\]
 then the same conclusion holds, with
\begin{align*}
U&\equiv (-\infty, \frac{(1-\eta)(K+1)}{2[2K+ (1-K)\eta]}
  \sqrt{\frac{(1+2\alpha)K-1+[2+\alpha (1-K)]\eta}{\beta [2K+(1-K)\eta]}})\\
&\quad  \cup  (-\frac{(1-\eta)(K+1)}{2[2K+ (1-K)\eta]}
  \sqrt{\frac{(1+2\alpha)K-1+[2+\alpha (1-K)]\eta}{\beta [2K+(1-K)\eta]}})
  ,\infty)
\end{align*}
 and $\mathcal{I}\equiv [-M,M]$ for $F\circ G$.
\end{lemma}

Now we try to set a period-doubling bifurcation theorem similar to
our  earlier work.

\begin{theorem}[Period-Doubling Bifurcation Theorem]
Let $\alpha$: $0<\alpha\le \frac{1}{K}$, $\beta >0$ be fixed, and let 
$\eta$: $0<\eta\le \underline{\eta}$ be a varying parameter. 
Let $h_1(v,\eta)=-G\circ F(v)$. Then

{\rm (i)} $v_0=
\frac{(K+1)(K+\eta)}{2[2K+(1-K)\eta]}\sqrt{\frac{(1 +2\alpha )K-1
+[2+\alpha(1-K)]\eta}{[2K+(1-K)\eta]\beta}}$
 is a curve of fixed points of $h_1$.

{\rm (ii)} The algebraic equation
\begin{equation} \label{algebraicEquation}
\begin{aligned}
&\frac{K-2K\alpha\eta+3\eta}{6\eta}\sqrt{\frac{1+\alpha\eta}{3\beta\eta}}\\
&= \frac{(K+1)(K+\eta)}{2[2K+(1-K)\eta]} \sqrt{\frac{(1 +2\alpha )K-1
+[2+\alpha(1-K)]\eta}{[2K+(1-K)\eta]\beta}}
\end{aligned}
\end{equation}
has a solution $\eta =\eta_0$ in $(0,1)$ for any given $\alpha$:
$0<\alpha \le \frac{1}{K}$ and $\beta >0$. We have
\[
\frac{\partial}{\partial v}h_1(v_0,\eta_0)=-1.
\]

{\rm (iii)} For $\eta =\eta_0$ satisfying \eqref{algebraicEquation}, we have
\begin{align*}
A&=\frac{\partial ^2}{\partial\eta\partial v}h_1
+\frac{1}{2}\frac{\partial h_1}{\partial \eta}\frac{\partial ^2h_1}{\partial v^2}\\
&=-\Big((K+1)\{[(K+1)\alpha(2\alpha+3)+3]\eta_0^3+(6K+\alpha
K+\alpha -3)\eta_0^2 \\
&\quad -(7K-2)\eta_0 +3K\}\Big)/\Big(3(1-\eta_0)^3(K+\eta_0)^2\Big).
\end{align*}
for $\eta=\eta_0$ and $v=v_0(\eta_0)$.

{\rm (iv)}
\begin{align*}
B&=\frac{1}{3}\frac{\partial ^3h_1} {\partial
v^3}+\frac{1}{2}(\frac{\partial ^2h_1}{\partial v^2})^2\\
&=\frac{8(K+1)\beta \eta^4}{(1-\eta_0)^2(K+\eta_0)^5}
\Big[(3\alpha -3K\alpha +1)\eta_0^3+(9K\alpha -3K^2\alpha-K+2)\eta_0^2\\
&\quad +K(6K\alpha-2K+7)\eta_0+5K^2\Big].
\end{align*}
\end{theorem}

\begin{proof}
 (i) This is an immediate consequence of Lemma \ref{Lemma2.3}.

 (ii) We first determine the point(s) $v>0$ such that
 $\frac{\partial h_1}{\partial v}=-1$. By \eqref{Derivative1},
 with a change of sign for $f_1$, we obtain
\[
\frac{K+\eta}{K(1-\eta)}[1-\frac{K+1}
{\frac{12K\beta}{(K+1)^2}g(v)^2+1-K\alpha}]=1.
\]
Therefore,
\begin{gather}
\frac{12K\beta}{(K+1)^2}g(v)^2=\frac{K}{\eta}+K\alpha, \notag \\
\label{Bifurcation1}
g(v)=\pm \frac{K+1}{2}\sqrt{\frac{1+\alpha\eta}{3\beta\eta}}.
\end{gather}
We choose positive $v$ and thus the ``$-$'' sign in \eqref{Bifurcation1}.
 Hence
\begin{align}\label{Bifurcation2}
g(v)=-\frac{K+1}{2}\sqrt{\frac{1+\alpha\eta}{3\beta\eta}}.
\end{align}
Since $g(v)$ satisfies \eqref{g}, from \eqref{Bifurcation2} we obtain
\begin{equation}\label{58}
\begin{aligned}
v&=-\frac{K}{K+1}[\frac{4\beta}{(K+1)^2}g(v)^3+(\frac{1}{K}-\alpha)g(v)]\\
&=\frac{K-2K\alpha\eta+3\eta}{6\eta}
\sqrt{\frac{1+\alpha\eta}{3\beta\eta}}\\
&= \text{LHS of   \eqref{algebraicEquation}}.
\end{aligned}
\end{equation}
Further setting \eqref{58} equal to $v_0(\eta)$ in (i), we obtain the
RHS of \eqref{algebraicEquation}.

Now we show that \eqref{algebraicEquation} has a solution. It is
easy to see that the LHS tends to $+ \infty$, but the RHS keeps
bounded as $\eta \rightarrow 0^{+}$. So the LHS is greater than the
RHS for some $\eta$ close to $0$. On the other hand, it is easy to
verify that the LHS is smaller than the RHS for some $\eta$ close to
$1$. It follows from the Mean Value Theorem of continuous functions
that \eqref{algebraicEquation} has a solution in $(0,1)$. (iii) and
(iv) are also immediate consequences of Lemma \ref{Lemma2.3}.
However, it is hard to judge whether $A\neq 0$ in (iii) and $B\neq
0$ in (iv) without knowledge of $\eta_0$. So we can not conclude the
period-doubling bifurcation so far. We will try other methods in
next section.
\end{proof}

\begin{theorem}[Homoclinic Orbits for the Case $0<\eta <1$]
Let $K>0$, $\alpha$: $0<\alpha \le \frac{1}{K}$ and $\beta >0$ be fixed, 
and let $\eta \in (0,1)$ be a varying parameter such that
\begin{align}
\frac{K+1}{2}\sqrt{\frac{1+\alpha}{\beta}}<\frac{K+\eta}{1-\eta}
\frac{1+\alpha}{3}\sqrt{\frac{1+\alpha}{3\beta}},\label{homoclinicCondition}
\end{align}
then the repelling fixed point $0$ of $G\circ F$ and $F\circ G$ has homoclinic
 orbits.
\end{theorem}

\begin{proof}
By \eqref{Derivative1} and \eqref{homoclinicCondition}, we easily obtain
\begin{align*}
\frac{\partial}{\partial v}f_i(v,\eta)|_{v=0}
&=\frac{K+\eta}{K(1-\eta)}(1-\frac{K+1}{1-K\alpha})\\
&=-\frac{(\alpha +1)(K+\eta)}{(1-\eta)(1-K\alpha)}
 < -1, \quad i=1,2.
\end{align*}
Therefore $0$ is a repelling fixed point of $G\circ F$ and $F\circ G$.
For a homoclinic to exist, the local maximum of $G\circ F$ (resp., $F\circ G$)
must be larger than the positive $v$-axis intercept of
$G\circ F$ (resp., $F\circ G$); i.e.,
\begin{align}
\frac{K+1}{2}\sqrt{\frac{1+\alpha}{\beta}}<\frac{K+\eta}{1-\eta}
\frac{1+\alpha}{3}\sqrt{\frac{1+\alpha}{3\beta}}.
\end{align}
This is exactly \eqref{homoclinicCondition}.
\end{proof}

\section{Klein-Gordon equation with variable coefficients}

In this section, we consider \eqref{KGeq1.15} with 
$a(x)\equiv Kb(x)$, where $K>0$ is a constant. 
Let $W=e^{-ct-d\eta}w$, where $w$ satisfies \eqref{2.1}. 
Then $w=e^{ct+d\eta}W$, and
\begin{gather*}
w_t=e^{ct+d\eta}(W_t+cW), \\
w_{\eta}=e^{ct+d\eta}(W_{\eta}+dW).
\end{gather*}
Then it follows immediately that
\begin{equation}\label{3.1}
[\frac{\partial}{\partial t}-K\frac{\partial}{\partial \eta}+c-Kd]
[\frac{\partial}{\partial t}+\frac{\partial}{\partial \eta}+c+d]W=0.
\end{equation}
Let $k_1=c-Kd$, $k_2=c+d$, then \eqref{3.1} becomes 
\begin{equation}\label{3.2}
[\frac{\partial}{\partial t}-a(x)\frac{\partial}{\partial x}+k_1]
[\frac{\partial}{\partial t}+b(x)\frac{\partial}{\partial x}+k_2]W=0.
\end{equation}
 Reversely, for any $k_1$ and $k_2$, there exist a unique pair of $c$ and $d$ 
such that $k_1=c-Kd$, $k_2=c+d$. Note that \eqref{3.2} is just our original
 problem \eqref{KGeq1.15}.

It follows immediately that
\[
\frac{1}{2}(w_{\eta}+w_t)=e^{ct+d\eta}
\frac{W_{\eta}+W_t+k_2W}{2} = c'_1,
\]
along each characteristics $ \eta +Kt=c_1$;
and
\[
\frac{1}{2}(Kw_{\eta}-w_t)=e^{ct+d\eta}\frac{KW_{\eta}-W_t-k_1W}{2} = c'_2,
\]
along each characteristics $\eta -t=c_2$.
Let
\begin{gather*}
u=\frac{W_{\eta}+W_t+k_2W}{2}=\frac{b(x)W_x+W_t+k_2W}{2},\\
v=\frac{KW_{\eta}-W_t-k_1W}{2}=\frac{a(x)W_x-W_t-k_1W}{2}.
\end{gather*}
 Then $e^{ct+d\eta}u$  keeps constant along lines $\eta +Kt=c$, and 
$e^{ct+d\eta}v$ keeps constant along lines $\eta -t=c$.

We impose boundary conditions such that
\begin{gather*}
v(0,t)  =G_{K,\lambda}(u(0,t))=\frac{K+\lambda}{1-\lambda}u(0,t), \\
u(1,t)  =F_{K,\alpha,\beta}(v(1,t)).
\end{gather*}
Then it is easy to deduce the corresponding boundary conditions:
\begin{gather}
W_t(0,t)
 =-\lambda b(0)W_x(0,t)-\frac{(1-\lambda)k_1+(K+\lambda)k_2}{K+1}W(0,t), \label{3.1leftboundary}
\\
\begin{aligned}
&\frac{(K+1)b(1)W_x(1,t)+(k_2-k_1)W(1,t)}{2}\\
& =\alpha \frac{(K+1)W_t(1,t)+(k_1+Kk_2)W(1,t)}{2} \\
&\quad -\frac{4\beta}{(K+1)^2}[\frac{(K+1)W_t(1,t)+(k_1+Kk_2)W(1,t)}{2}]^3\,.
\end{aligned} \label{3.1rightboundary}
\end{gather}
It is easy to verify the following reflective iterations:
\begin{gather}
u(1,t)  =F(G(e^{-(1+\frac{1}{K})cL}u(1,t-L-\frac{L}{K})),\label{reflection3.1} \\
v(0,t)  =G(e^{(d-\frac{c}{K})L}F(e^{-(c+d)L}v(0,t-L-\frac{L}{K})).\label{reflection3.2}
\end{gather}

\begin{lemma}[Solution representations for $u(x,t)$ and $v(x,t)$]\label{Lemma3.1}
Assume \eqref{3.1}, \eqref{3.1leftboundary} and \eqref{3.1rightboundary}. 
Then for any $x$: $0<x<1$, and $t>0$, we have, for $t=(1+\frac{1}{K})jL+\tau$, 
$j=0,1,2,\dots$, $\tau >0$,
\begin{gather*}
u(x,t) = \begin{cases}
\big(F(G(e^{-(1+\frac{1}{K})cL}\cdot))\big)^j 
\Big(F(e^{-(c+d)(\tau-\frac{L-\eta}{K})}v_0(\psi^{-1}(1+\frac{1}{K})L
-\tau-\frac{\eta}{K}))\Big), \\
\quad \text{if } L\le K\tau +\eta \le (K+1)L;
\\[4pt]
\big(F(G(e^{-(1+\frac{1}{K})cL}\cdot))\big)^j 
\Big(F_{\alpha,\beta}\Big(e^{-(c+d)L}G(e^{(Kd-c)
(\tau+\frac{\eta}{K}-(1+\frac{1}{K})L)}\\
\times u_0(\psi^{-1}(K\tau+\eta-(K+1)L)))\Big)\Big),\\
\quad \text{if } (K+1)L \le K\tau +\eta \le (K+2)L;
\end{cases}
\\[4pt]
v(x,t) =\begin{cases}
\big(G(e^{(d-\frac{c}{K})L}F(e^{-(c+d)L}\cdot))\big)^j 
\Big(G\Big(e^{(Kd-c)(\tau-\eta)}u_0(\psi^{-1}(K(\tau-\eta)))\Big)\Big),\\
\quad \text{if } 0\le \tau -\eta \le \frac{L}{K};
\\[4pt]
\big(G(e^{(d-\frac{c}{K})L}F(e^{-(c+d)L}\cdot))\big)^j 
\Big(Ge^{(d-\frac{c}{K})L}F\Big(e^{-(c+d)(\tau-\eta-\frac{L}{K})}\\
\times v_0(\psi^{-1}
((1+\frac{1}{K})L-\tau+\eta))\Big)\Big), \\
\quad \text{if } \frac{L}{K} \le \tau -\eta \le (1+\frac{1}{K})L.
\end{cases}
\end{gather*}
\end{lemma}

Over all, the dynamics of $u$ and $v$ are determined by iterative
compositions of functions $f_1$ and $f_2$ as:
\begin{gather*}
f_1(v,\eta)
=G_{\eta}(e^{(d-\frac{c}{K})L}F(e^{-(c+d)L}v))
=\frac{K+\eta}{1-\eta}e^{(d-\frac{c}{K})L}F(e^{-(c+d)L}v)),
\\
f_2(v,\eta)=F(G(e^{-(1+\frac{1}{K})cL}v))
=F(\frac{K+\eta}{1-\eta}(e^{-(1+\frac{1}{K})cL}v)),
\end{gather*}
where $F=F_{K,\alpha,\beta}$ is as defined in previous section.

The proof of bifurcations depend on the analysis of the derivatives
of $f_1$ or $f_2$ with respect to $v$ and $\eta$. One can imagine
that it is a hard work, since the formulations of $f_1$ and $f_2$
are so complicated.

 Chaos and bifurcations are determined by the
reflection maps $F(G(e^{-(1+\frac{1}{K})cL}\cdot))$ or
$G(e^{(d-\frac{c}{K})L}F(e^{-(c+d)L}\cdot))$. Since the
 two maps are conjugate to each other, it suffices to
consider either one of them.

 Let us look at $F(G(e^{-(1+\frac{1}{K})cL}\cdot))$. Given $\alpha$, 
$\beta$ and $K$, $F$ is fixed, then the map varies with
 $G(e^{-(1+\frac{1}{K})cL}\cdot)$. In a word, the dynamics depend on the 
value of $\frac{K+\lambda}{1-\lambda}e^{-(1+\frac{1}{K})cL}$. 
So it may be reasonable to define the factor as a parameter.
Let $\eta = \frac{K+\lambda}{1-\lambda}e^{-(1+\frac{1}{K})cL}$, 
then the reflective map $f_2$ can be simplified as
\begin{align}
f_2(v)=F_{\alpha,\beta,K}(\eta v).
\end{align}
Of course, it should be much easier to calculate the derivatives 
of $f_2$ with respect to $v$ and the new parameter $\eta$, 
so we will easily get the regime of $\eta$ where $f_2$ is chaotic or bifurcated. 
Then the corresponding regime of $\lambda$ can be obtained by simple calculations. 
Let us do it as follows:

\begin{lemma}[Derivative Formulas]\label{DerivativeFormulas}
Let  $0<\alpha\le \frac{1}{K}$, $\beta >0$ and $\eta \in \mathbb{R}$, 
where $\alpha$ and $\beta$ are given and fixed, but $\eta$ is a varying parameter. 
Define $f(v,\eta)=F_{\alpha,\beta,K}(\eta v)$, $v\in \mathbb{R}$.
Let $g(v)$ be the unique real solution of the cubic equation
\begin{equation}
\frac{4\beta}{(K+1)^2}g(v)^3+(\frac{1}{K}-\alpha)g(v)+(\frac{1}{K}+1)v=0,
\end{equation}
for a given $v\in \mathbb{R}$.
Then
\begin{itemize}
\item[(i)] $\frac{\partial}{\partial v}f(v,\eta)
 =\eta\frac{12\beta g(\eta v)^2-(\alpha +1)(K+1)^2}{12K\beta g(\eta v)^2+(1-K\alpha)(K+1)^2}$,
\item[(ii)] $\frac{\partial}{\partial \eta}f(v,\eta)
 =v\frac{12\beta g(\eta v)^2-(\alpha +1)(K+1)^2}{12K\beta g(\eta v)^2+(1-K\alpha)(K+1)^2}$,
\item[(iii)] $\frac{\partial^2}{\partial \eta \partial v}f_(v,\eta)
 =\frac{12\beta g(\eta v)^2-(\alpha +1)(K+1)^2}{12K\beta g(\eta v)^2+(1-K\alpha)(K+1)^2}-\frac{24\beta (K+1)^6\eta g(\eta v)v}{[12K\beta g(\eta v)^2+(1-K\alpha)(K+1)^2]^3}$,
\item[(iv)] $\frac{\partial^2}{\partial v^2}f(v,\eta)
 =-\frac{24\beta (K+1)^6\eta ^2g(\eta v)}{[12K\beta g(\eta v)^2+(1-K\alpha)(K+1)^2]^3}$,
\item[(v)] $\frac{\partial^3}{\partial v^3}f(v,\eta)
 =-24\beta (K+1)^9\eta ^3\frac{60K\beta g(\eta v)^2-(1-K\alpha)(K+1)^2}{[12K\beta g(\eta v)^2+(1-K\alpha)(K+1)^2]^5}$.
 \end{itemize}
\end{lemma}


\begin{lemma}[Intersections with the Lines $u-v=0$ and $u+v=0$]
\label{LemmaUVIntersects}
Let $\alpha$: $0<\alpha\le \frac{1}{K}$, $\beta >0$, $\eta \in\mathbb{R}$ be given. 
Then

{\rm (i)} If $\eta >K$ or $\eta <-\frac{1-K\alpha}{1+\alpha}$, then
$u=f(v)$ intersects the line $u=v$ at the points
\[
 (u,v)=(-\frac{K+1}{2(\eta -K)}\sqrt{\frac{1-K\alpha 
+(\alpha +1)\eta}{\beta(\eta -K)}},
   -\frac{K+1}{2(\eta -K)}\sqrt{\frac{1-K\alpha +(\alpha +1)\eta}{\beta(\eta -K)}}),
\]
(0,0), 
\[
 (\frac{K+1}{2(\eta -K)}\sqrt{\frac{1-K\alpha +(\alpha +1)\eta}{\beta(\eta -K)}},
   \frac{K+1}{2(\eta -K)}\sqrt{\frac{1-K\alpha +(\alpha +1)\eta}{\beta(\eta -K)}});
\]

{\rm (ii)} If $\eta <-K$ or $\eta >\frac{1-K\alpha}{1+\alpha}$, then
$u=f(v)$ intersects the line $u=-v$ at the points
\[
 (u,v)=(-\frac{K+1}{2(\eta +K)}\sqrt{\frac{(\alpha +1)\eta 
+\alpha K-1}{\beta(\eta +K)}},
   \frac{K+1}{2(\eta +K)}\sqrt{\frac{(\alpha +1)\eta +\alpha K-1}{\beta(\eta +K)}}),
\]
$(0,0)$, 
\[
(\frac{K+1}{2(\eta +K)}\sqrt{\frac{(\alpha +1)\eta +\alpha K-1}{\beta(\eta +K)}},
   -\frac{K+1}{2(\eta +K)}\sqrt{\frac{(\alpha +1)\eta +\alpha K-1}{\beta(\eta +K)}}).
\]
\end{lemma}

\begin{lemma}[$v$-aixs Intercepts]\label{vAxisIntercept}
Let $\alpha$: $0<\alpha\le \frac{1}{K}$, $\beta >0$, $\eta >0$, $\eta \neq 1$
 be given. Then 
 $u=f(v)$ has $v$-axis intercepts
\[
v=-\frac{K+1}{2\eta}\sqrt{\frac{1+\alpha}{\beta}}, \quad
0,  \quad
\frac{K+1}{2\eta}\sqrt{\frac{1+\alpha}{\beta}}.\]
 \end{lemma}

\begin{lemma}[Local Maximum, Minimum and Piecewise Monotonicity]\label{localM} 
Let $\alpha$: \\ 
$0<\alpha\le \frac{1}{K}$, $\beta >0$, $\eta \in \mathbb{R}$ be given. 
Then  If $\eta >0$, then $f$ has local extremal values
\begin{gather*}
M=f(-v_c)=\frac{1+\alpha}{3}\sqrt{\frac{1+\alpha}{3\beta}}, \\
m=f(v_c)=-\frac{1+\alpha}{3}\sqrt{\frac{1+\alpha}{3\beta}},
\end{gather*}
where $v_c=\frac{3+(1-2\alpha)K}{6\eta}\sqrt{\frac{1+\alpha}{3\beta}}$, 
and $M$, $m$ are, respectively, the local
   maximum and minimum of $f$. The function $f$ is strictly increasing on 
$(-\infty, -\tilde{v}_c)$ and $(\tilde{v}_c, \infty)$, 
but strictly decreasing on $(-\tilde{v}_c, \tilde{v}_c)$.

   On the other hand, if $\eta<0$, then $f$ has local extremal values
\begin{gather*}
m=f(-v_c)=-\frac{1+\alpha}{3}\sqrt{\frac{1+\alpha}{3\beta}}, \\
M=f(v_c)=\frac{1+\alpha}{3}\sqrt{\frac{1+\alpha}{3\beta}}.
\end{gather*}
The function $f$ is strictly decreasing on $(-\infty, -v_c)$ and 
$(v_c, \infty)$, but strictly increasing on $(-v_c, v_c)$.
\end{lemma}

\begin{lemma}[Bounded Invariant Intervals]\label{boundedInvariantInterval}
Let $0<\alpha\le 1/K$, $\beta >0$, $\eta \in \mathbb{R}$.

{\rm (i)} If $\eta >K$, and
$$
\frac{1+\alpha}{3}\sqrt{\frac{1+\alpha}{3\beta}}<\frac{K+1}{2(\eta -K)}
\sqrt{\frac{1-K\alpha +(\alpha +1)\eta}{\beta(\eta -K)}},
$$
then the iterates of every point in the set
\begin{align*}
U&\equiv (-\infty,-\frac{K+1}{2(\eta -K)}
 \sqrt{\frac{1-K\alpha +(\alpha +1)\eta}{\beta(\eta -K)}})\\
&\quad \cup (\frac{K+1}{2(\eta -K)}\sqrt{\frac{1-K\alpha +(\alpha +1)\eta}
{\beta(\eta -K)}},\infty)
\end{align*}
 escape to $\pm \infty$, while those of any point in $\mathbb{R}\backslash \bar{U}$ 
are attracted to the bounded invariant interval ${\mathcal{I}}\equiv [-M,M]$ of $f$;

{\rm (ii)} If $\eta <-K$, and
 $$
\frac{1+\alpha}{3}\sqrt{\frac{1+\alpha}{3\beta}}
<-\frac{K+1}{2(\eta +K)}\sqrt{\frac{(\alpha +1)\eta +\alpha K-1}{\beta(\eta +K)}},
$$
 then the iterates of every point in the set
\begin{align*}
U&=(-\infty,\frac{K+1}{2(\eta +K)}\sqrt{\frac{(\alpha +1)\eta 
+\alpha K-1}{\beta(\eta +K)}})\\
&\quad \cup (-\frac{K+1}{2(\eta +K)}\sqrt{\frac{(\alpha +1)\eta +\alpha K-1}
{\beta(\eta +K)}},\infty)
\end{align*}
 escape to $\pm\infty$, while those of any point in  $\mathbb{R}\backslash \bar{U}$ 
are attracted to the bounded invariant interval ${\mathcal{I}}\equiv [-M,M]$ of $f$.
\end{lemma}

\begin{theorem}[Period-Doubling Bifurcation Theorem]\label{periodDoublingBifurcation}
Let $K>0$, $\alpha$: $0<\alpha\le \frac{1}{K}\le 2\alpha +1$, $\beta
>0$ be fixed, and let $\eta$: $\eta >0$ be a varying parameter. Then

{\rm (i)} For $0<\eta <\frac{1-K\alpha}{1+\alpha}$,
$0$ is the unique fixed point of $f$, and it is stable;

{\rm (ii)} With the same $\alpha$, $\beta$ and $K$ as in (i),
but $\eta >\frac{1-K\alpha}{1+\alpha}$, then $0$ becomes unstable,
and there appear stable period-$2$ orbit 
\[
\big\{\frac{K+1}{2(\eta +K)}\sqrt{\frac{(\alpha +1)\eta +\alpha K-1}{\beta(\eta
+K)}},-\frac{K+1}{2(\eta +K)}\sqrt{\frac{(\alpha +1)\eta +\alpha
K-1}{\beta(\eta +K)}}\big\}
\]
 of $f$;

{\rm (iii)} The curve of the period-$2$ points:
$$
v=\pm\frac{K+1}{2(\eta +K)}\sqrt{\frac{(\alpha +1)\eta +\alpha K-1}
{\beta(\eta +K)}}
$$
 is smooth in the $\eta$-$v$ plane,
and tangent to the line $\{\frac{1-K\alpha}{1+\alpha}\}\times \mathbb{R}$ 
at point $(\frac{1-K\alpha}{1+\alpha},0)$;

{\rm (iv)} The period-$2$ orbit becomes unstable when $\eta$ increases 
through 
\[
\frac{K+1+\sqrt{(K+1)^2-(\alpha +1)(1-K\alpha)K}}{\alpha +1}.
\]
\end{theorem}

\begin{proof}
 (i) It follows from Lemma \ref{DerivativeFormulas} (i) that
\begin{align*}
f'(0) 
& =\eta\frac{12\beta g(0)^2-(\alpha +1)(K+1)^2}{12K\beta g(0)^2+(1-K\alpha)(K+1)^2}\\
& =\eta\frac{-(\alpha +1)(K+1)^2}{(1-K\alpha)(K+1)^2}\\
& =-\eta \frac{\alpha +1}{1-K\alpha}.
\end{align*}
So
$-1<f'(0)<0$,
for $0<\eta <\frac{1-K\alpha}{1+\alpha}$. So the origin point is a
stable fixed point of $f$. As is shown in Lemma
\ref{LemmaUVIntersects}, there are no other fixed points of $f$ when
$0<\eta <\frac{1-K\alpha}{1+\alpha}\le K$, so $0$ is the unique
fixed point of $f$.

 (ii) Let
\begin{align*}
v_0=\frac{K+1}{2(\eta +K)}\sqrt{\frac{(\alpha +1)\eta +\alpha K-1}{\beta(\eta +K)}};
\end{align*}
i.e., the positive intersection of $f$ with the line $u=-v$.
Then
\begin{gather*}
F(\eta v_0)=-v_0, \\
\frac{\eta v_0+g(\eta v_0)}{K}=-v_0, \\
g(\eta v_0)=-(K+\eta)v_0.
\end{gather*}
So
\[
g(\eta v_0)^2
 =(\eta +K)^2v_0^2
 =\frac{(K+1)^2[(\alpha +1)\eta +\alpha K-1]}{4\beta (\eta +K)}.
\]
Furthermore,
\begin{equation} \label{3.15}
\begin{aligned}
\frac{\partial f}{\partial v}|_{v=v_0}
& =\eta\frac{12\beta \frac{(K+1)^2[(\alpha +1)\eta +\alpha K-1]}{4\beta (\eta +K)}
 -(\alpha +1)(K+1)^2}{12K\beta \frac{(K+1)^2
 [(\alpha +1)\eta +\alpha K-1]}{4\beta (\eta +K)}+(1-K\alpha)(K+1)^2} \\
& =\eta \frac{3[(\alpha +1)\eta+\alpha K-1]-(\alpha +1)(\eta +K)}
 {3K[(\alpha +1)\eta +\alpha K-1]+(1-K\alpha)(\eta +K)} \\
& =\eta \frac{2(\alpha +1)\eta +2\alpha K-K-3}{(2\alpha K+3K+1)\eta +2(\alpha K-1)K}.
\end{aligned}
\end{equation}
On the other hand,
\[
2(\alpha +1)\eta +2\alpha K-K-3  >2(1-\alpha K)+2\alpha K-K-3 >-K-1,
\]
and thus
\begin{equation}
|2(\alpha +1)\eta +2\alpha K-K-3|<K+1 \label{3.16}
\end{equation}
for $\eta $ greater than $\frac{1-\alpha K}{\alpha +1}$ and close to
$\frac{1-\alpha K}{\alpha +1}$ enough,
\begin{equation}
\begin{aligned}
& (2\alpha K+3K+1)\eta +2(\alpha K-1)K \\
& =2K(\alpha +1)\eta +(K+1)\eta +2(\alpha K-1)K \\
& >2K(1-\alpha K)+(K+1)\eta +2(\alpha K-1)K \\
& >(K+1)\eta ,
\end{aligned}\label{3.17}
\end{equation}
for $\eta $ greater than $\frac{1-\alpha K}{\alpha +1}$.

Combining \eqref{3.15}, \eqref{3.16} and \eqref{3.17}, we have
\[
|f'(v_0)|<1
\]
for $\eta $ greater than $\frac{1-\alpha K}{\alpha +1}$ 
and close to $\frac{1-\alpha K}{\alpha +1}$ enough.
 By similar arguments we have
\[
|f'(-v_0)|<1
\]
for $\eta $ greater than $\frac{1-\alpha K}{\alpha +1}$ and close to
 $\frac{1-\alpha K}{\alpha +1}$ enough.

Combining the two aspects above, we conclude that the new emerging
period-$2$ orbit ares stable. This completes the proof of the
period-$2$ bifurcations of $f$ at the origin.

(iii) It is easy to verify that 
\[
v=\pm\frac{K+1}{2(\eta +K)}\sqrt{\frac{(\alpha +1)\eta +\alpha K-1}{\beta(\eta +K)}}
\]
 is differentiable with respect to $\eta$ for $\eta $ in 
$(\frac{1-\alpha K}{\alpha +1}, \infty)$.
 The derivative is $\infty$ at $\eta =\frac{1-\alpha K}{\alpha +1}$. 
This shows that the curve is smooth in the $\eta$-$v$ plane, and tangent
 to line $\{\frac{1-K\alpha}{1+\alpha}\}\times \mathbb{R}$ at point 
$(\frac{1-K\alpha}{1+\alpha},0)$.

(iv) Let
\[
 \frac{\partial f}{\partial v}=\eta \frac{2(\alpha +1)\eta +2\alpha K-K-3}
{(2\alpha K+3K+1)\eta +2(\alpha K-1)K}>1,
\]
 and then it follows that
\[
 \eta >\frac{K+1+\sqrt{(K+1)^2-(\alpha +1)(1-\alpha K)K}}{\alpha +1},
\]
 or
\[
 \eta <\frac{K+1-\sqrt{(K+1)^2-(\alpha +1)(1-\alpha K)K}}{\alpha  +1}.
\]
 So the period-$2$ orbit becomes unstable when $\eta$ increases through 
\[
\frac{K+1+\sqrt{(K+1)^2-(\alpha +1)(1-\alpha K)K}}{\alpha +1}.
\]
\end{proof}

\begin{remark} \label{rmk3.1} \rm
We just conclude that $0$ is stable by $|f'(0)|<1$ when $0<\eta <
\frac{1-K\alpha}{1+\alpha}$. However, $|f'(0)|<1$ just implies the
local stability of $0$. In fact, it follows from Lemma
\ref{LemmaUVIntersects} that
 $u=f(v)$ does not intersect with line $u=v$ or $u=-v$
 at other points except the origin, so we have
$|f(v)|<|v|$ for $v \neq 0$. Therefore, $0$ attracts $(-\infty,
+\infty)$, illustrated by Figure \ref{globalAttract}:

\begin{figure}[ht]
\begin{center}
\includegraphics[width=0.7\textwidth]{fig3-1}
\end{center} %  0Attract.eps
\caption{Global attraction diagram of $0$ for $f$, where $\alpha=0.5$, $\beta=1$,
$K=0.7$, $\eta=0.4$.} \label{globalAttract}
\end{figure}
\end{remark}

\begin{remark} \label{rmk3.2} \rm
The stable period-$2$ orbit in Theorem
\ref{periodDoublingBifurcation} (ii) attracts $(-\infty,0)\cup
(0,+\infty)$ for $\eta$ larger than and close to
$\frac{1-K\alpha}{1+\alpha}$. Since $-f(-f(v))=f(f(v))$, so the
period-$2$ stability under $f$ is equivalent to that under $-f$. The
global attraction of its period-$2$ orbit can be easily illustrated
by its graph, e.g., Figure \ref{Fig.3.2}.
\end{remark}

\begin{figure}[ht]
\begin{center}
\includegraphics[width=0.7\textwidth]{fig3-2}
\end{center} % period2.eps 
\caption{Global attraction diagram of the period-$2$ orbit for $f$, where
$\alpha=0.5$, $\beta=1$, $K=0.7$, $\eta=0.8$.} \label{Fig.3.2}
\end{figure}



\begin{theorem}[Homoclinic Orbits for the Case $\eta >0$]
\label{HomoclinicOrbits} Let $K>0$, $\alpha$: $0<\alpha \le 1/K$ and $\beta >0$
 be fixed, and $\eta \geq \frac{3\sqrt{3}(K+1)}{2(1+\alpha)}$,
  then the repelling fixed point $0$ of $f$ has homoclinic orbits.
\end{theorem}

\begin{proof}
For a homoclinic orbit of $0$ to exist, the local maximum of $f$
must be no less than the positive $v$-axis intercept of $f$, i.e.,
\[
\frac{K+1}{2\eta}\sqrt{\frac{1+\alpha}{\beta}}
<\frac{1+\alpha}{3}\sqrt{\frac{1+\alpha}{3\beta}},
\]
which is equivalent to
\begin{equation}
\eta > \frac{3\sqrt{3}(K+1)}{2(1+\alpha)}.\label{homoclinicOrbitCondition}
\end{equation}
On the other hand, it follows from Lemma \ref{DerivativeFormulas} (i) that
\[
\frac{\partial}{\partial v}f(v,\eta)|_{v=0}
=-\eta\frac{\alpha +1}{1-K\alpha}.
\]
Therefore $0$ is a repelling fixed point of $f$ for $\eta$ larger
 than $\frac{1-K\alpha}{\alpha +1}$, which is implied by
\eqref{homoclinicOrbitCondition}.
This completes the proof.
\end{proof}

For $\eta =\frac{3\sqrt{3}(K+1)}{2(1+\alpha)}$, $v_c$ (or $-v_c$)
lies on a degenerated homoclinic orbit. When
$\eta <\frac{3\sqrt{3}(K+1)}{2(1+\alpha)}$, $f$
has maximum less than the $v$-axis intercept.
Hence there are no points homoclinic to $0$ for these $\eta$-values.
 On the other hand, when $\eta >\frac{3\sqrt{3}(K+1)}{2(1+\alpha)}$,
 there are infinitely many distinct homoclinic orbits.
 Consequently, $f$ is not structurally stable when
 $\eta =\frac{3\sqrt{3}(K+1)}{2(1+\alpha)}$, i.e.,
 a small change in $f$ can change the number of homoclinic orbits.

\begin{example} \label{examp3.1} \rm
The parameters chosen are
$\alpha=0.5$, $\beta=1$, $\lambda=0.85$, $k_1=k_2=0.7$, $K=0.7$, $b(x)=1+3x^2$,
$$
w(x,0)=\sin^2(\pi x), \quad w_t(x,0)=0.
$$
Figures \ref{Fig3.3}--\ref{Fig3.6} show the spatiotemporal profiles of 
$u$, $v$, $w_x$ and $w_t$ for $x\in [0,1]$ and
$t\in [7.34,8.80]$ respectively; Figures \ref{Fig3.7} and \ref{Fig3.8} 
illustrate the reflection maps $F(G(e^{-(1+\frac{1}{K})cL}\cdot))$ and 
$G(e^{(d-\frac{c}{K})L}F(e^{-(c+d)L}\cdot))$ respectively.
\end{example}

\begin{figure}[ht]
\begin{center}
\includegraphics[width=0.8\textwidth]{fig3-3}
\end{center} % fig3_1.eps
\caption{The spatiotemporal profile of $u(x,t)$ for $x\in [0,1]$ and $t\in [7.34,
8.80]$.} \label{Fig3.3}
\end{figure}

\begin{figure}[ht]
\begin{center}
\includegraphics[width=0.8\textwidth]{fig3-4}
\end{center} % fig3_2.eps
\caption{The spatiotemporal profile of $v(x,t)$ for $x\in [0,1]$ and $t\in
[7.34,8.80]$.} \label{Fig3.4}
\end{figure}

\begin{figure}[ht]
\begin{center}
\includegraphics[width=0.8\textwidth]{fig3-5}
\end{center} % fig3_3.eps
\caption{The spatiotemporal profile of $w_x(x,t)$ for $x\in [0,1]$ and $t\in
[7.34, 8.80]$.} \label{Fig3.5}
\end{figure}

\begin{figure}[ht]
\begin{center}
\includegraphics[width=0.8\textwidth]{fig3-6}
\end{center} % fig3_4.eps
\caption{The spatiotemporal profile of $w_t(x,t)+kw(x,t)$ for $x\in [0,1]$ and
$t\in [7.34, 8.80]$.} \label{Fig3.6}
\end{figure}

\begin{figure}[ht]
\begin{center}
\includegraphics[width=0.7\textwidth]{fig3-7}
\end{center} % fig3_5.eps
\caption{Orbits of $H_1=F(G(e^{-(\frac{k_1}{K}+k_2)L}\cdot))$, $\alpha=0.5$, $\beta=1$,
$\lambda=0.85$, $k_1=k_2=0.7$, $K=0.7$.} \label{Fig3.7}
\end{figure}

\begin{figure}[ht]
\begin{center}
\includegraphics[width=0.7\textwidth]{fig3-8}
\end{center} % fig3_6.eps
\caption{Orbits of $H_2=G(e^{-\frac{k_1}{K}L}F(e^{-k_2L}\cdot))$, $\alpha=0.5$,
$\beta=1$, $\lambda=0.85$, $k_1=k_2=0.7$, $K=0.7$.} \label{Fig3.8}
\end{figure}

Figures \ref{Fig3.7} and \ref{Fig3.8} show that $H_1$ and $H_2$
are topologically transitive, so probably they are chaotic
according to Devaney's definition \cite{Saber}.

\section{Period doubling bifurcation and pitchfork bifurcation
route to chaos}

The mapping $f_{\eta}$ (or $H_1$, $H_2$) has a unique fixed point or
periodic point ($0$), which is stable when $\eta>0$ is small enough.
As $\eta$ increases, the fixed point $0$ becomes unstable, and there
appears a stable periodic-$2$ orbit, then the period-$2$ orbit
becomes unstable, too. Finally, homoclinic orbits appear when $\eta$
is large enough. We have proved these facts in Theorem
\ref{periodDoublingBifurcation} and \ref{HomoclinicOrbits}. In this
section, we try to explore more about the bifurcation routes.

Let us start by a bifurcation diagram, we take $\alpha=0.5$,
$\beta=1$, $K=0.7$, and let $\eta$ vary from $0.4$ to $3$.
 The stable fixed point $0$ bifurcates into a
stable symmetric period-$2$ orbit at $\eta \approx 0.43$, then the
symmetric period-$2$ orbit bifurcates into two new stable period-$2$
orbits at $\eta \approx 2.2$, then they bifurcate into two
period-$4$ orbits at $\eta \approx 2.6$. The bifurcations are
illustrated by Figures \ref{Fig.4.1} and \ref{Fig.4.2}. To distinguish
the pitchfork period-$2$ bifurcation from the period doubling
bifurcation of period-$4$, we start our iteration at $v=0.3$ and
$v=-0.3$ respectively, and found that they are stablized by
different period-$2$ orbits.

It is easy to see that there is a pitchfork bifurcation of
period-$2$ following the period doubling bifurcation of period-$2$
described by Theorem \ref{periodDoublingBifurcation}.


\begin{figure}[ht]
\begin{center}
\includegraphics[width=0.7\textwidth]{fig4-1}
\end{center}  % fenchatu1.eps
\caption{Bifurcation diagram of $f$, where $\alpha=0.5$, $\beta=1$,
$K=0.7$, iteration starts at $v=0.3$.} \label{Fig.4.1}
\end{figure}

\begin{figure}[ht]
\begin{center}
\includegraphics[width=0.7\textwidth]{fig4-2}
\end{center}  % fenchatu2.eps
\caption{Bifurcation diagram of $f$, where $\alpha=0.5$, $\beta=1$,
$K=0.7$, iteration starts at $v=-0.3$.} \label{Fig.4.2}
\end{figure}

Let us compare this experiment results with Theorem \ref{periodDoublingBifurcation}.

$\bullet$ The first bifurcation: from the fixed point to period-$2$ orbit.
According to Theorem \ref{periodDoublingBifurcation} (i)-(ii), the
first bifurcation parameter value is
\begin{align}\label{bifurcationParameter1}
\eta = \frac{1-K\alpha}{1+\alpha}.
\end{align}
Substitute the experiment parameter values $\alpha=0.5$ and $K=0.7$
to \eqref{bifurcationParameter1}, we obtain
\begin{align*}
\eta=\frac{1-K\alpha}{1+\alpha}=0.4333,
\end{align*}
 which agrees with the bifurcation diagrams.

$\bullet$ The second bifurcation:
 from the symmetric period-$2$ orbit to the nonsymmetric period-$2$ orbits.
According to Theorem \ref{periodDoublingBifurcation} (iv),
 the second bifurcation parameter value is 
\begin{align}\label{secondBifurcation}
\eta = \frac{K+1+\sqrt{(K+1)^2-(\alpha +1)(1-K\alpha)K}}{\alpha +1}.
\end{align}
Substitute the experiment parameters to \eqref{secondBifurcation},
we obtain $\eta =2.1238$, which agrees with the bifurcation
diagrams.

The \emph{ old} period-$2$ points
 $\pm\frac{K+1}{2(\eta +K)}\sqrt{\frac{(\alpha +1)\eta +\alpha K-1}
 {\beta(\eta +K)}}$ of $f$ are fixed points of $-f$.
 Suppose $-f$ has a period-doubling bifurcation at
\[
\eta=\frac{K+1+\sqrt{(K+1)^2-(\alpha +1)(1-K\alpha)K}}{\alpha +1},
 \]
 then the period-$2$ orbits of $-f$ are just the \emph{ new}
  period-$2$ orbits of $f$.
Let us check it as follows.

\begin{proof}
   Let $h=-f$, we have found the parameter value and the fixed point
   for which $\frac{\partial h}{\partial v} =-1$.
   So it suffices to verify that
\begin{gather*}
   A\equiv \Big[\frac{\partial ^2h}{\partial\eta\partial v}
+\frac{1}{2}(\frac{\partial h}{\partial\eta})\frac{\partial^2h}{\partial v^2} \Big]
\neq 0, 
\\
   B\equiv \frac{1}{3}\frac{\partial^3h}{\partial v^3}
   +\frac{1}{2}(\frac{\partial^2h}{\partial v^2})^2\neq 0,
\end{gather*}
 for
   \begin{gather}\label{periodTwoPoint}
   v= v_0\triangleq \frac{K+1}{2(\eta +K)}
\sqrt{\frac{(\alpha +1)\eta +\alpha K-1}{\beta(\eta +K)}}, \\
\label{periodTwoParameter}
    \eta= \eta_0\triangleq \frac{K+1+\sqrt{(K+1)^2-(\alpha +1)(1-K\alpha)K}}{\alpha +1}.
\end{gather}
It follows from Theorem \ref{DerivativeFormulas} that
\begin{equation}
\begin{aligned}
A
&=-\frac{12\beta g(\eta_0 v_0)^2-(\alpha +1)(K+1)^2}{12K\beta
g(\eta_0 v_0)^2+(1-K\alpha)(K+1)^2} \\
&\quad +\frac{24\beta (K+1)^6\eta_0 g(\eta_0 v_0)v_0}{[12K\beta g(\eta_0 v_0)^2
  +(1-K\alpha)(K+1)^2]^3} \\
&\quad -\frac{12\beta (K+1)^6\eta_0 ^2g(\eta_0 v_0)v_0
 [12\beta g(\eta_0 v_0)^2-(\alpha +1)(K+1)^2]}
 {[12K\beta g(\eta_0 v_0)^2+(1-K\alpha)(K+1)^2]^4}, \label{A}
\end{aligned}
\end{equation}
and
\begin{align*}
B&=8\beta(K+1)^9\eta_0^3\frac{60K\beta
g(\eta_0v_0)^2-(1-K\alpha)(K+1)^2}{[12K\beta
g(\eta_0v_0)^2+(1-K\alpha)(K+1)^2]^5}\\
&\quad +\frac{288\beta^2(K+1)^{12}\eta_0^4g(\eta_0v_0)^2}{[12K\beta
g(\eta_0v_0)^2+(1-K\alpha)(K+1)^2]^6}.
\end{align*}
Combing Theorem \ref{DerivativeFormulas} (i) and the fact that
$\frac{\partial f}{\partial v} =1$ for $\eta=\eta_0$, $v=v_0$, we
have
\[
12\beta g(\eta_0 v_0)^2-(\alpha +1)(K+1)^2>0.
\]
Noting that $g(\eta v)$ and $v$ have opposite sign, so all the terms
in the RHS of \eqref{A} are negative. Therefore $A<0$.

By similar arguments we have $B>0$. This completes the proof.
   \end{proof}

The \emph{ old} period-$2$ orbit $\{p(\eta), -p(\eta)\}$ becomes unstable
 after the second bifurcation,
 and a pair of stable period-$2$ orbits appear.
 Denote them by $\{p_1(\eta) ,q_1(\eta)\}$
 and $\{p_2(\eta) ,q_2(\eta)\}$ respectively,
 where $p_1$ and $p_2$ are around $p$, $q_1$ and $q_2$
 are around $-p$. Let
\[
 p_1>p,\quad  p_2<p.
\]
 Then
\[
 q_1>-p,\quad  q_2<-p,
\]
 since $f$ is increasing around $p$ and $-p$.
  This pair of stable period-$2$ orbits can be illustrated by
Figure \ref{Fig.4.1} and Figure \ref{Fig.4.2} (curves over
$\eta\in (2.12,2.55)$).

Let us look at the period-$4$ bifurcation. By period doubling
bifurcation theorems, it occurs where $\frac{\partial }{\partial
v}(f\circ f)|_{v=p_i}=f'(p_i)f'(q_i)=-1$, $i=1,2$.

On the other hand,
\[
\frac{\partial }{\partial v}(f\circ f)=f'(p)f'(-p)=1
\]
at the pitchfork bifurcation point of period-$2$.
Since $\frac{\partial }{\partial v}(f\circ f)$ varies continuously
with respect to parameters and arguments, so
$\frac{\partial }{\partial v}(f\circ f)$ must vanish
 at some period-$2$ point before period-$4$ bifurcation.
Since $\frac{\partial }{\partial v}(f\circ f)=0$ if and only if the
period-$2$ cycle contains extremal point $v_c$ or $-v_c$, the
extremal point $v_c$ or $-v_c$ must be contained in a period-$2$
orbit before period-$4$ bifurcation.
This process can be illustrated
by the following experiment results and figures:

We take $\alpha=0.5$, $\beta=1$, $K=0.7$, $\eta=1.8$, then Theorem
\ref{periodDoublingBifurcation} (ii) tells that the unique symmetric
period-$2$ orbit is $\{0.3079,-0.3079\}$. Figure \ref{Fig.4.3}
illustrates this fact.

\begin{figure}[ht]
\begin{center}
\includegraphics[width=0.7\textwidth]{fig4-3}
\end{center} %symmetryPeriod2.eps
\caption{Stable symmetric period-$2$ orbit of $f$,
 where $\alpha=0.5$, $\beta=1$, $K=0.7$, $\eta=1.8$.}
 \label{Fig.4.3}
\end{figure}

Then we take larger $\eta=2.2$, the symmetric period-$2$ orbit
bifurcates into two branches of stable period-$2$ orbits,
illustrated by Figure \ref{Fig.4.4}.

\begin{figure}[ht]
\begin{center}
\includegraphics[width=0.7\textwidth]{fig4-4}
\end{center} %twoPeriod2.eps
\caption{Two branches of stable period-$2$ orbits of $f$, where $\alpha=0.5$,
$\beta=1$, $K=0.7$, $\eta=2.2$.}\label{Fig.4.4}
\end{figure}

Take $\eta=2.3$, the two branches of period-$2$ orbits go apart, and
pass by the extremal points, illustrated by Figure \ref{Fig.4.5}
\begin{figure}[ht]
\begin{center}
\includegraphics[width=0.7\textwidth]{fig4-5}
\end{center} % passVc.eps
\caption{Two branches of period-$2$ orbits of $f$,
 where $\alpha=0.5$, $\beta=1$, $K=0.7$, $\eta=2.3$,
 period-$2$ orbits pass by extremal points $\pm  v_c$.}\label{Fig.4.5}
\end{figure}

Take $\eta=2.6$, each period-$2$ orbit bifurcates into a stable
period-$4$ orbit, illustrated by fig. \ref{Fig.4.6}.

\begin{figure}[ht]
\begin{center}
\includegraphics[width=0.7\textwidth]{fig4-6}
\end{center} % twoPeriod4.eps
\caption{Two branches of stable period-$4$ orbits of $f$, where $\alpha=0.5$,
$\beta=1$, $K=0.7$, $\eta=2.6$.}\label{Fig.4.6}
\end{figure}

It is well known that a discrete dynamical system is chaotic if it
has a homoclinic orbit. According to Theorem \ref{HomoclinicOrbits},
$f$ has homoclinic orbits and chaos when $\eta \geq
\frac{3\sqrt{3}(K+1)}{2(1+\alpha)}$. For $\alpha =0.5$ and $K=0.7$,
the condition is as $\eta \geq 2.9445$, which agrees with
bifurcation diagrams Figure \ref{Fig.4.1} and Figure \ref{Fig.4.2}.

In addition to homoclinic orbits, period three is a classical
criteria for chaos. 

\begin{theorem}\label{periodThree}
Given $\alpha$, $\beta$ and $K$, there exists $\eta_3$ such that
$F(\eta_3\cdot)$ has period $3$.
\end{theorem}

\begin{proof}
It is easy to verify that $F(\bar{\eta}\cdot)$ has period three,
where $\bar{\eta}$ is the critical value of $\eta$ such that the local
maximum equals to the positive intercept with line $u=v$.
 Let $d=M$,
$c=-v_c$, $b\in (0,v_c)$ such that
\begin{equation}
F(\bar{\eta}b)=-v_c,
\end{equation}
and $a\in (v_c,M]$ such that
\begin{equation}
F(\bar{\eta}a)=b.
\end{equation}
It is easy to see that $c<b<a<d$. Then the period three follows from
the Li-York's Theorem.
\end{proof}

\begin{remark} \label{rmk4.1} \rm
By continuity, there exists $a\in (v_c,M]$ such that
\[
 f_{\eta}^2(a)<f_{\eta}(a)<a<f_{\eta}^3(a)
\]
for $\eta$ around $\bar{\eta}$. So $f_{\eta}$ has period three for
$\eta$ in a neighbor of $\bar{\eta}$. This is why we often see 
\emph{Period Three Windows} in bifurcation diagrams. Of course, a rigorous
proof must include the stability of the period-$3$ orbits in the
\emph{ window}, e.g., an extremal point is in one of the period-$3$
cycles. We omit the rigorous proof here.
\end{remark}

We give the period-$3$ orbit for $\alpha=0.5$, $\beta=1$, $K=0.7$
and $\eta=4.1$ in Figure \ref{Fig.4.7}.

\begin{figure}[ht]
\begin{center}
\includegraphics[width=0.7\textwidth]{fig4-7}
\end{center} % period3.eps
\caption{The period-$3$ orbit of $f$, where $\alpha=0.5$, $\beta=1$, $K=0.7$,
$\eta=4.1$.}\label{Fig.4.7}
\end{figure}

We give the bifurcation diagram of $f$ for $\alpha =0.5$, $\beta =1$
and $\eta \in [3.5, 4.1]$ in Figure \ref{Fig.4.8}.  Two windows of
period-$6$ seem emerge, over $\eta =3.77$ and $3.92$ respectively.

\begin{figure}[ht]
\begin{center}
\includegraphics[width=0.8\textwidth]{fig4-8}
\end{center} % window3.eps
\caption{The bifurcation diagram of $f$, where $\alpha=0.5$, $\beta=1$, $K=0.7$,
$\eta \in [3.5, 4.1]$. Two windows of period-$6$ seem
emerge.}\label{Fig.4.8}
\end{figure}


\section{A more general case}

Let $W=e^{-ct-\int_0^{\eta}d(\eta)d\eta}w$, where $d(\eta)$ is a real function 
defined on $[0,L]$, and $w$ satisfies \eqref{2.1}. 
Then $w=e^{ct+\int_0^{\eta}d(\eta)d\eta}W$, and
\begin{gather*}
w_t=e^{ct+\int_0^{\eta}d(\eta)d\eta}(W_t+cW), \\
w_{\eta}=e^{ct+\int_0^{\eta}d(\eta)d\eta}(W_{\eta}+d(\eta)W).
\end{gather*}
Then it follows immediately that
\begin{equation}\label{4.1}
[\frac{\partial}{\partial t}-K\frac{\partial}{\partial \eta}+c-Kd(\eta)]
[\frac{\partial}{\partial t}+\frac{\partial}{\partial \eta}+c+d(\eta)]W=0,
\end{equation}
or
\begin{equation}\label{4.2}
[\frac{\partial}{\partial t}-a(x)\frac{\partial}{\partial x}+c-Kd(\psi(x))]
[\frac{\partial}{\partial t}+b(x)\frac{\partial}{\partial x}+c+d(\psi(x))]W=0.
\end{equation}
Let $k_1(x)=c-Kd(\psi(x))$, $k_2(x)=c+d(\psi(x))$, then
\begin{equation}\label{4.3}
[\frac{\partial}{\partial t}-a(x)\frac{\partial}{\partial x}+k_1(x)]
[\frac{\partial}{\partial t}+b(x)\frac{\partial}{\partial x}+k_2(x)]W=0.
\end{equation}

On the other hand, given $k_1(x)$ and $k_2(x)$, assume that
$k_1(x)+Kk_2(x)$ is a constant. Then
\[
d(\eta)=\frac{-k_1(\psi^{-1}(\eta))+k_2(\psi^{-1}(\eta))}{K+1},\quad 
c=\frac{k_1+Kk_2}{K+1}.
\]
Let
\[
u=\frac{1}{2}[b(x)W_x+W_t+k_2(x)W], \quad 
v=\frac{1}{2}[a(x)W_x-W_t-k_1(x)W].
\]

\begin{lemma}[Constancy along characteristics]
\begin{equation} \label{KGeq3.8}
\begin{gathered}
e^{ct+\int_0^{\eta}d(\eta)d\eta}u = c'_1,\quad \text{along each characteristic }
  \eta+Kt=c_1,\\
e^{ct+\int_0^{\eta}d(\eta)d\eta}v = c'_2,\quad \text{along each characteristic }
  \eta-t=c_2.
\end{gathered}
\end{equation}
\end{lemma}

We impose boundary conditions
\begin{gather*}
W_t(0,t)+cW(0,t)=-\lambda [b(0)W_x(0,t)+d(0)W(0,t)],\\
b(1)W_x(1,t)+d(L)W(1,t) =\alpha [W_t(1,t)+cW(1,t)]-\beta
[W_t(1,t)+cW(1,t)]^3,
\end{gather*}
and obtain the following result.

\begin{lemma}[Composite reflection relations]
\begin{gather*}
u(1,t) = F_{\alpha,\beta,K}(G_\lambda(e^{-(1+\frac{1}{K})cL}u(1,t-(1+\frac{1}{K})L))),
\\
v(0,t) = G_\lambda(e^{\int_0^Ld(\eta)d\eta-c\frac{L}{K}}
F_{\alpha,\beta}(e^{-cL-\int_0^Ld(\eta)d\eta}v(0,t-(1+\frac{1}{K})L))),
\end{gather*}
for any $t>0$.
\end{lemma}

Then the dynamics of $u$ and $v$ are determined by the iterative
compositions of
$F_{\alpha,\beta,K}(G_\lambda(e^{-(1+\frac{1}{K})cL}\cdot))$ and
$G_\lambda(e^{\int_0^Ld(\eta)d\eta-c\frac{L}{K}}
F_{\alpha,\beta}(e^{-cL-\int_0^Ld(\eta)d\eta}\cdot))$.

\subsection*{Acknowledgements}
This research was supported by  grant \#NPRP 4-1162-1-181 from the
from the Qatar National Research Fund (a member of Qatar
Foundation). 

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\end{document}
