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{\bigtype
\quad
\vskip.5cm
\centerline{\bf Equilibrium States for Lattice Models of Hyperbolic Type}}
\vskip.3cm
\centerline{ M{$\!\!$\smalltype IAOHUA} \ J$\!\!${\smalltype IANG} 
%\footnote {${}^{}$}{\medtype{\ 
%%%%%%%%%
%insert footnotes below
%%%%%%%%
\qquad
%}}
}
{\smedtype
\centerline{\it Department of Mathematics}
\centerline{\it The Pennsylvania State University}
\centerline{\it University Park,    PA 16802}
}


\vskip1.5cm
 

\medtype

 
\centerline{\bf  Abstract} 

 We study the structural stability of coupled map lattice models  of  
hyperbolic 
type under certain metrics. We prove the existence of equilibrium states for
continuous functions  on lattice models under the
conditions of weak interaction and translation invariance. We also study the
 uniqueness and ergodic properties of these equilibrium states for  H\"older
 continuous functions.  

AMS classification: 58F11, 58F15, 34D30, 34C35
\vskip.8cm
\centerline{ \bf 1. INTRODUCTION }
\vskip.1cm
Let $M$ be a compact Riemannian manifold  and $U \subset M$ an open set.
Let $f: U \to M $ be a $C^{1 + \alpha}$-diffeomorphism   and let $\Lambda 
\subset U $ be a closed invariant {\it hyperbolic set} for $f$. This means 
that the 
tangent bundle $TM$ has a splitting ({\it exponential splitting}) into 
subbundles
 over $\Lambda$: \ $TM=E^s \bigoplus E^u$
, where $E^s, E^u$ are both invariant under the differential  $Df$, and for 
some $0<\lambda < 1$,
$$\| Df^n v\| \leq C \lambda^n \|v\| \hbox{\rm \ for} \ n\geq 0, v \in E^s;$$
$$\| Df^{-n} w\| \leq C \lambda^n \|w\| \hbox{\rm \ for} \ n\geq 0, w \in E^u.
$$
The hyperbolic set $\Lambda$ is called {\it locally maximal} if there 
exists an 
open set $O \contain \Lambda$ such that 
$ \Lambda = \cap_{n \in \integer} f^n(\bar O)$.
 The dynamics on any compact  locally maximal hyperbolic set is semiconjugate 
to a {\it subshift of finite type} and there exist  invariant
measures ( {\it equilibrium states}) that have abundance of  ergodic
properties. Each of these measures is uniquely defined by a {\it H\"older 
continuous}
function on $\Lambda$.  

Starting from the diffeomorphism $f$, one can consider an space extended  
 infinite dimensional dynamical system $F= \otimes_{i \in \integer} f$ 
and consider a
small perturbation $\Phi$ of $F$ on $ \MM= \otimes_{i \in \integer} M$. 
It is called
a {\bf lattice model}. The iteration of the map $\Phi$ generates a group
 of time translations. An important class of lattice models consists of  
those that also admit a group of {\it space translations} (see the 
definition below).  Such models were considered  in [BS] in the case 
when $f$ is a one-dimensional expanding map, and in [PS] in the case 
 when $f$ possesses
a {\it hyperbolic attractor} (i.e., there exists an open neighborhood $U
 \contain \Lambda$ such that $\overline{f(U)} \subset U$ and $\Lambda = 
\cap_{n \geq 0} f^n(U)$). In both cases, the authors constructed  
analogues of {\it SBR measures} that are equilibrium states for
 certain functions.       In this  paper, we  consider the dynamics 
of lattice models in a more general situation when
 the  dynamical system $f$ possesses a hyperbolic set. We prove 
structural stability of  lattice dynamical system $F$  under different 
 metrics and  existence of   equilibrium states for  continuous functions.
    We also study the uniqueness  and the ergodic properties of these 
measures with respect to both space and time translations for   H\"older
 continuous functions. The above  problems were also considered in   
[GR1], [GR2], [GR3], and [CR].  However, many statements in these
 papers are incorrect, the proofs presented in these papers   have 
 many gaps. The 
main result (Theorem 1) of the second paper in the series  that claims
 the uniqueness of Gibbs states for H\"older continuous functions   
is actually wrong. A class of  counterexamples is provided by the Ising
 model in statistical physics (see [MM]).


\vskip.8cm
\centerline{\bf 2. DEFINITION OF LATTICE MODELS}

   We begin with the description of   lattice models. 
Define $$\MM =  \otimes_{i \in \integer} M_i = 
                 \{ \bar x \  |\  \bar x = (x_i), x_i \in M\},$$  where 
 $M_i$ is  a copy
of $M$.

We endow  $\MM$  with a  {\it Finsler metric} so that $\MM$ becomes a
 differentiable Banach
manifold modeled on $(\Rn)^{\integer}$. Let $\bar x =(x_i) \in \MM$ 
and $(V_i,
\phi_i)$ be charts around $x_i \in M$ for each $i$. Then, a  chart
 containing $\bar x$ will be: $ (\otimes_{i \in \integer}V_i, 
\otimes_{i \in \integer} \phi_i)$. Let $\xi_i \in T_{x_i}M_i$. Then 
$\bar \xi =(\xi_i) \in T_{\bar x}\MM$ and
$$ \| \bar \xi\| = \sup_{i \in \integer}\|\xi_i\|.$$
Let $\bar x, \bar y$ be two points in $\MM$. The distance on $\MM$ 
induced by the Finsler metric is:
$$\rho(\bar x, \bar y)= \sup_{i \in \integer} d(x_i,y_i),$$ where
$d$ is the Riemannian distance on $M$.


The definition of hyperbolicity can be easily extended to  Banach 
manifolds.
Suppose that $G$ is a $C^1$-diffeomorphism from an open set of a Banach
 manifold
$\NN$ with a Finsler metric and $\Delta_G$ is an invariant set under $G$.
 We say
that $\Delta_G$ is a (uniformly) hyperbolic set if the tangent bundle
$T\NN$ over
$\Delta_G$ has a splitting: $T\NN = E^s \oplus E^u$ with the following 
properties: {\sl
\item{1)}  $E^s, E^u$ are invariant under $DG$;
\item{2) } for any continuous sections $v$ valued of $E^s$ and  $w$ of 
$E^u$ 
$$\|DG^n( v)\| 
        \leq C \lambda^n  \| v\| \quad \hbox{\rm and} \quad \|DG^{-n}( w)\| 
       \leq C \lambda^n  \| w\|$$ for some constants $C>0$  and $0<\lambda<1$
independent of $v$ and $w$;
\item{3)}  there exists $b>0$ such that for any $\bar x = (x_i)$,
$$\inf \{ \|\xi - \eta\| : \xi \in E^s(\bar x), \| \xi \| =1;  \eta
 \in E^u(\bar x), \| \eta \|=1 \} \ge b.$$
}

Define $F= \otimes_{i \in \integer}f$. It  is a diffeomorphism of $\MM$
of class $C^{1+\alpha}$. The closed set $\Delta = \otimes_{i \in \integer}
\Lambda_i,$ $ \Lambda_i = \Lambda,$  is   invariant under $F$ and hyperbolic.
 For each point $\bar x =(x_i) \in \Delta$, the tangent space $T_{\bar x}\MM$ 
admits a splitting:  $T_{\bar x}\MM =E^s(\bar x) \oplus E^u(\bar x),\ 
\hbox{\rm where} \quad E^s(\bar x) = \otimes_{i \in \integer}E^s(x_i)
\ \  \hbox{\rm and }\  E^u(\bar x) = \otimes_{i \in \integer}E^u(x_i).$ 
  The subbundles $
E^s(\bar x), E^u(\bar x)$ are invariant under the differential $DF= 
\otimes_{i \in \integer}Df $, and for any $\bar v =(v_i) \in E^s(\bar x)$
 and $\bar w =(w_i) \in E^u(\bar x)$ 
$$\|DF^n(\bar v)\|= \sup_{i \in \integer}\|Df^n(v_i)\| 
        \leq C \lambda^n \sup_{i \in \integer}\|v_i\|= C \lambda^n  \|\bar v\|
$$
and
$$\|DF^{-n}(\bar w)\|=\sup_{i \in \integer}\|Df^{-n}(w_i)\| 
   \leq C \lambda^n \sup_{i \in \integer}\|w_i\|= C \lambda^n  \|\bar w\|,$$
where $C$ is a constant and $0<\lambda<1$. Without loss of generality, 
by switching to another equivalent
Riemannian metric and replacing $\lambda$ by a big constant $\lambda_1 <1 $
 we may  assume $C=1$. 
       

For each point $\bar x = (x_i)_{i \in \integer} \in \Delta$, let  $V_i^s(x_i)$
 and $V_i^u(x_i)$ be the local stable and unstable manifolds respectively at
 $x_i$. The local stable and unstable manifolds passing through $\bar x $ are
$$ V^s(\bar x) = \otimes_{i \in \integer}V_i^s(x_i), \qquad
V^u(\bar x) = \otimes_{i \in \integer}V_i^u(x_i).$$ 
  One  can  obtain the global stable and unstable
manifolds in a similar way.

The distance between two mappings on $\MM$ is defined as usual: If
$G$ and $G'$  are two $C^1$ diffeomorphism of $\MM$, then
$$ \dist_{C^0}(G,G') = \sup_{\bar x \in \MM} \rho(G(\bar x), G'(\bar x));$$
$$\dist_{C^1}(G,G') = \sup_{\bar x \in \MM} \rho(G(\bar x)), G'(\bar x))
+ \sup_{\bar x \in \MM}\|DG_{\bar x}-DG'_{\bar x}\|.$$
Let  $G: \MM \to \MM$ be a map $C^{1}-$close to the identity  $id$.  We 
define the perturbation $\Phi = F \cdot G$. Let $S$ be the left shift
({\it space translation} ) on $\MM$ defined by $ (S(\bar x))_i  = x_{i+1}$. 
The pair $(\Phi, S)$ is called a {\bf lattice model}.


\vskip.8cm
\centerline{\bf 3. MAIN RESULTS}

{\bf 3.1 \  Structural Stability} \quad We first consider the problem of 
structural stability  of the infinite dimensional hyperbolic system  
($\MM, F$). 

{\bf Theorem 1} \qquad {\sl
1)  There exist a neighborhood $U(\Delta) \supset \Delta$ and $\delta_0 >0$ 
such that if  $ \dist_{C^1}(\Phi, F) \leq \delta_0$, then any subset 
$\Delta_{\Phi} \subset U(\Delta)$  invariant under $\Phi$ is  uniformly 
hyperbolic.

2)  For any $\eps >0$, there exists $0 <\delta< \delta_0 $ such that if
 $ \dist_{C^1}(\Phi, F) \leq \delta$, then there is a unique homeomorphism 
$h: \Delta \to \MM$ 
satisfying $\Phi \cdot h = h \cdot F$ with $\dist_{C^0}(h, id) \leq \eps$.}
 
This theorem    is well-known for finite dimensional dynamical systems. 
It can also be stated for general hyperbolic  systems on
 Banach manifolds that admit the partition of unity. 
The dynamical system  ($\MM, F$) we consider  does not admit such a property 
and the general result can not be applied in a direct way. However this 
system is a direct product of countable many  copies of the same compact 
Riemannian manifold $M$. This special structure    enables us to present
 the proof of the theorem that is modeled on the proof in the finite 
dimensional case in [KH] and [Sh].
 

In the following theorem we study the  topological  properties of map 
$\Phi$ on the hyperbolic set
$\Delta_{\Phi}$.



{\bf Theorem 2}\qquad {\sl Assume that $f|_{\Lambda}$ is topologically 
mixing and
$\Lambda$ is locally maximal. Then $\Phi|_{\Delta_{\Phi}}$ is topologically
 mixing
and $\Delta_{\Phi}$ is locally maximal. }

{\bf 3.2 \  Short Range Mappings}\quad 
The main goal of this article is to investigate the metric properties of
 the  above infinite dimensional hyperbolic systems.  In the finite 
dimensional case,
one uses  the {\it thermodynamic formalism } [Bo] [Ru] to study the 
ergodicity of maps on hyperbolic sets. The extension of this formalism
 to infinite dimensional case  is tricky since the hyperbolic set $ \Delta$
 is not compact. We overcome this problem by introducing the following
family of metrics  on the
manifold $\MM$. 


 We
define the metric $\rho_q$, $0<q<1$, as follows: for $\bar x, \bar y \in \MM$ 
$$\rho_q(\bar x, \bar y) = \sup_{i \in \integer} q^{|i|} d(x_i,y_i).$$
For different $0<q<1$, the metrics $ \rho_q$ induce the same compact topology
on $\MM$. Thus in this new topology the set $\Delta$ is compact. However, 
 the set $\Delta$  is no longer  hyperbolic in the usual sense with respect
to   the  coarser  metric $\rho_q$. The set $\MM$ is not  a differential
 manifold  and the  maps $F$ and $ \Phi$, while being continuous, need
 not be differentiable. 

We will  restrict our perturbations to a smaller class of maps that are
 called {\bf short range mappings}.  This concept  arises naturally from 
 statistical mechanics. The short range  mappings were first considered
 by Bunimovich and Sinai  in the one-dimensional case [BS] (see also [KF]),
   and were later investigated by Pesin and Sinai  in a more general
 situation [PS] (see also [GR1] [CR]).  Our definition of a short range
 mapping below follows that in [PS].

    Let $Y$ be a subset of $\MM$.


{\bf Definition}\quad  {\sl 1)   A mapping $G: Y \to \MM $ is called 
 {\bf a short range mapping} if $G$ has the form  $G=(\cdots, G_{-n}, 
\cdots,G_{-1},G_0, G_1, \cdots,G_n, \cdots)$, where
$G_i,  Y \to M_i, i \in \integer$, satisfies the following condition:
 for any fixed $k \in \integer$
and any  points $\bar x =(x_j), \bar y=(y_j) \in Y$ with $x_j=y_j$ for all
$j \in \integer, j\not=k$, we have
$$d(G_i(\bar x), G_i(\bar y)) \leq C \theta^{|i-k|} d(x_k,y_k),$$
where $C$ and $\theta$ are constants and $0<\theta<1$. We shall call $\theta$
the {\bf decay constant} of $G$.

2) A mapping $G$ is called {\bf shift invariant}
if $G \cdot S = S \cdot G.$ \hb Let $G= (\cdots, G_{-n}, \cdots,G_{-1},G_0,
 G_1, \cdots,G_n, \cdots) $.   One can easily see that 
  $G$ is  shift invariant if and only 
if $G_i = G_0 \cdot S^i, i \in \integer,$ }
 where $S$ is the left shift
on $\MM$.
If $G$ is  shift invariant, then $G$   is  short ranged with a decay constant
 $\theta$ if and only if
$$d(G_0(\bar x), G_0(\bar y)) \leq C \theta^{|k|} d(x_k,y_k)$$
for $\bar x =(x_j), \bar y=(y_i) \in Y$ with $x_j=y_j$ for all
$j \in \integer, j\not=k$.
 

We formulate some basic properties of  short range mappings.


{\bf Lemma 1}\qquad  1) Let $G: \MM \to \MM$ be a short range mapping with 
a decay constant $\theta$. Then 
  it is Lipschitz continuous as a map from $(\MM, \rho_{q})$ to itself for
 any $q > \theta$. 

2) If   $G$ is a Lipschitz continuous  map from $(\MM, \rho_{q})$ to  
$(\MM, \rho_{q_1})$, with some $0< q_1 < 1$,  then it is  short ranged with
the decay constant $\theta$ equal to $q$.


{\bf Lemma 2} \qquad Let $G$ be a $C^1$-diffeomorphism from an open set 
$\UU \subset \MM$ onto its image. Then, the following statements are 
equivalent.

1) \quad The mapping $G$ is  short ranged with a decay constant $\theta$.

2) \quad  The differential of $G$ at $\bar x$, $D_{\bar x}G : T_{\bar x}\MM \to
T_{\bar x}\MM $ is a short range linear mapping with the same decay constant 
$\theta$ which is independent of  ${\bar x}$.

3) \quad The bundle map $DG$ is  short ranged  with the same decay constant 
$\theta$.

{\bf  Lemma 3}\qquad For any $0< \theta < 1$, there exists $\eps > 0$ such 
that if
$G : \MM \to \MM$ is a short range $C^{1+\alpha}$-diffeomorphism  with the 
decay constant $\theta$ and
$ \hbox{\rm dist}_{C^1}(G, id ) < \eps$, then $G^{-1}$ is also a short range
mapping.



{\bf Lemma 4}\qquad  For any $\eps > 0$  and  $0 < \theta < q<1 $ there
exist $\delta$ such that if $G$ is a $C^{1+\alpha}$ shift invariant short
 range
mapping on $\MM$ with the decay constant $\theta$ and 
 $ \dist_{C^1}(G, id ) \leq \delta,$
 then
$G$ is Lipschitz continuous on $\MM$ in the metric $\rho_q$ with a Lipschitz
 constant $L \leq 1+ \eps$.




Note that $F^{-1}$,  the inverse of the unperturbed map $F$ is Lipschitz
continuous in the metric $\rho_q$ on the local unstable manifold 
$\otimes V^u(\bar x)$ with a Lipschitz
constant $L = \lambda < 1$. As an easy corollary of the previous lemma, one
can see that   the inverse of the perturbed map $\Phi= F \cdot G$ \ 
$\Phi^{-1}$ is
also Lipschitz continuous in the  metric   $\rho_q$ with a Lipschitz 
constant $L = (1+\eps) \lambda$ on $\otimes V^u(\bar x).$  We will fix 
an $\eps$ so  that $(1+\eps) \lambda <1 $.





In Theorem 1, we proved that  $(\Delta, \FF)$ and $(\Delta_{\Phi},\Phi)$ are 
conjugate hyperbolic systems. One can prove that the conjugacy $h$ is  H\"older
 continuous. However, we need another property of $h$ that is related to the
 metric $\rho_q$. The following theorems, which use the above lemmas,  show
 that when the perturbation is short ranged, the conjugacy $h$ is  continuous
 in the  metric $\rho_q,$
 and that if $G$ is $C^2$, the conjugacy map $h$ is
 actually H\"older continuous
 in the metric $\rho_q$.


{\bf Theorem 3}\qquad Let $\Phi = F \cdot G$ be the perturbation of $F$. If
 the map $G$ is  short ranged and sufficiently $C^1$-close to the identity,
 then the  conjugacy $h$   is also   continuous in the metric $\rho_q$, hence,
it is  a homeomorphism  between $\Delta$ and $\Delta_{\Phi}$. Moreover, if $G$
 is shift invariant, so is $h$.



{\bf Theorem 4}\qquad For any  $0<\theta <1 $ 
there exists  $\delta >0$
such that if $G$ is a $C^{2}-$shift invariant short ranged  mapping  
 with the decay constant $\theta$ and 
 $\dist_{C^1}(G, id) \leq \delta,$
then  the conjugacy map $h$  is
H\"older continuous in the metric $\rho_q, \  0< q <1.$ 





{\bf 3.3  \ Existence of Equilibrium States} \quad
  Let $\Omega$ be a compact metric space, $\tau$  a
$\integer^2-$action on $\Omega$ induced by a pair of commutative 
 homeomorphisms. Let $\UU=\{ U_i\}, \BB=\{ B_i\}$ be covers of $\Omega$. 
The cover
$\UU \vee \BB$ consists of the sets $U_i \cap B_j$. For a finite set
$X \subset \integer^2$, define
$$ \UU^X = \vee_{x \in X} \tau^{-x}\UU.$$


{\bf Definitions}\ [Ru]\qquad
{\sl 1. A $\integer^2-$action $\tau$ is said to be {\bf expansive} if
 there exists $\epsilon >0$ 
such that for any $\xi, \eta \in \Omega,$ 
$$ d(\tau^x \xi, \tau^x \eta) \leq \epsilon \hbox{ \rm \  for\ all } 
x \in \integer^2 \hbox{\rm \  implies \ } \xi = \eta$$
for any $\xi, \eta \in \Omega.$

2. A Borel measure $\mu$ on $\Omega$  is said to be $\tau$-{\bf invariant} if 
$\mu$ is invariant under both homeomorphisms.  We denote the set of
all $ \tau$-invariant measure on $\Omega$ by $I(\Omega)$.

3. Let $\mu \in I(\Omega)$ and $\UU = \{ U_i\}$ be any finite Borel partition
 of $\Omega$
. Define
$$H(\mu,\UU)= - \sum_{i}\mu(U_i)\log \mu(U_i)$$ and
$$h_{\tau}(\mu, \UU)= \lim_{(n,m)\to \infty} {1 \over nm}H(\mu,\UU^{X_{nm}})
                 = \inf_{n,m} {1 \over nm}H(\mu,\UU^{X_{nm}}),$$where 
$ X_{nm}=\{ (i,j) \in \integer | \ |i| \leq n, |j| \leq m\} $.
The {\bf entropy} of $\mu$ is defined to be
$$h_{\tau}(\mu)= \sup_{\UU}h_{\tau}(\mu, \UU)= \lim_{diam\UU \to 0} h_{\tau}
(\mu, \UU).$$

4. Let $\UU$ be any finite open cover of $\Omega$,   $\varphi$ a continuous
function on $\Omega$, and  $X$  a finite subset of $\integer^2$. Define
$$Z_{X}(\varphi, \UU) = \min_{\{B_j\}}\big\lbrace \sum_j  \exp\big\lbrack 
\inf_{\xi \in B_j}
\sum_{x \in X} \varphi (\tau^x \xi)\big\rbrack\big\rbrace,$$ where the minimum 
is taken over all 
subcovers $\{B_j\}$ of $\UU^X$. Let
$$P_{\tau}(\varphi,\UU)= 
\limsup_{(n,m) \to \infty} {1 \over nm} \log Z_{X_{nm}}
(\varphi, \UU).$$
Then 
$$ P_{\tau}(\varphi)= \lim_{diam\UU \to 0} P_{\tau}(\varphi,\UU) =
\sup_{\UU}P_{\tau}(\varphi,\UU)$$ is called the  {\bf topological pressure}
of $\varphi$.

5. A measure $\mu \in I(\Omega)$ is called an {\bf equilibrium state} for 
$\varphi$ on $\Omega$
with respect to a $\integer^2$ action $\tau$ if 
$$P_{\tau}(\varphi)= h_{\tau}(\mu) + \int \varphi d\mu.$$
}

{\bf Proposition 1 }[Ru] \qquad {\sl   If $\tau$ is an expansive
 $\integer^2$-action on a compact
metric space, then there exists an equilibrium state for any continuous 
function $\varphi.$ }



The existence of equilibrium states on $\Delta_{\Phi}$ for  continuous 
functions $\varphi$ follows directly  from the above proposition   and Theorems
 3 since
the $\integer^2-$action induced by $(\Phi, S)$ is expansive on 
$(\Delta_{\Phi}, \rho_q)$.

{\bf Theorem 5 } \qquad {\sl  Let $\tau$ be the $\integer^2-$action  on 
$\Delta_{\Phi}$ induced by $\Phi$ and
$S$, where $\Phi= F\cdot G $ and $G$ is short ranged, shift invariant  
 and sufficiently $C^1-$close to identity. Then
for any $0<q<1$ and any continuous function $\varphi$ on  $(\Delta_{\Phi},
\rho_q)$ there exists
an equilibrium state $\mu_{\varphi}$ for $\varphi$ with respect to $\tau$.
 The measure $\mu_{\varphi}$ does not depend on $q$.}


{\bf 3.4 \  Uniqueness of Equilibrium States.}\quad
Following the general scheme that was used  in the finit-dimensional case,
we study the uniqueness of equilibrium states for H\"older continuous 
functions using symbolic dynamics. First we  construct
a {\bf Markov partition} for $\Phi$ on $\Delta_{\Phi}$. Since 
$(\Delta_{\Phi}, \Phi)$ is
conjugate to $(\Delta, F)$, we     construct a Markov partition on 
$\Delta$ and then transform it   to a Markov partition on $\Delta_{\Phi}$ 
using the
conjugating map $h$.

 We shall assume that $f$ is topologically mixing and $\Lambda$ is
locally maximal.
For any $\eps > 0$, there exists  a Markov partition of ``size'' $\eps$ of 
 $\Lambda$ for $f$:
 $\Lambda =\cup_{i=1}^m R_i$. This means that  

1) each set $R_i$ is a ``{\it rectangle}'', i.e., for any $x,y \in R_i,
 \ V^s(x) \cap V^u(y) \in R_i$,  $ diamR_i < \eps$,  $R_i$ is the closure 
of its interior, i.e.,  $R_i=
\overline {(int R_i)}$.

2)  $R_i \cap R_j = \partial R_i \cap \partial  R_j$, where $\partial R_i$
 denotes the boundary of $R_i$.

3)  if $x \in R_i$ and $f(x) \in int R_j$, then $f(V^s(x, R_i)) \subset 
V^s(f(x), R_j)$; if $x \in R_i$ and $f^{-1}(x) \in int R_j$, then
 $f^{-1}(V^u(x, R_i)) \subset 
V^u(f(x), R_j)$, where $ V^s(x, R_i) = V^s(x)\cap R_i$ and $V^u(x, R_i)
 = V^u(x)\cap R_i.$

The transfer matrix $A=(a_{ij})_{1 \leq i,j \leq m}$ associated with 
the Markov
partition is defined by 
$$ a_{ij} =1 \ \hbox{\rm if}\  f(int R_i) \cap int R_j \not= \emptyset;$$
$$ a_{ij} =0 \ \hbox{\rm if}\  f(int R_i) \cap int R_j = \emptyset.$$
Let $(\Sigma_A, \sigma)$ be the   associated subshift of finite type, 
where $\sigma$ is the left shift on $\Sigma_A$.   For each $\xi \in \Sigma_A$,
 the set $\cap_n f^{-n}(R_{\xi(n)})$ contains a single point and the map 
$\pi: \Sigma_A \to \Lambda$ defined by $\pi{\xi} = \cap_nf^{-n}(R_{\xi(n)})$
 is a semiconjugacy between $f$ and   $\sigma$ on . Denote   $m^{\integer} 
= \otimes_{i \in \integer} \{1,2, \cdots, m \}$, 
  $R_{(n_i)}=\{\bar x : \bar x= (x_i), x_i \in R_{n_i}, n_i\in 
\{ 1,2, \cdots,m\} \}$. Then $\Delta= \cup_{(n_i) \in m^{\integer}} R_{\xi(n)}$
 and   the collection of subsets of $\Delta$, $\{ R_{(n_i)} : (n_i) \in 
m^{\integer} \}, $ has the following properties:

1)   each   $ R_{(n_i)}$ is a closed set in both the Finsler topology and 
the
product topology and for any $\bar x, \bar y \in \Delta$, $ \ V^s(\bar x) 
\cap V^u(\bar y) \in R_{(n_i)}$.

2)   $ F( V^s(\bar x, R_{(n_i)}) ) \subset V^s(F(\bar x), R_{(m_i)})$ and  
$ F^{-1}( V^u(F(\bar x), R_{(n_i)}) ) $ \hb $ \subset V^u(\bar x, R_{(m_i)})$, 
where $ V^{s,u}(\bar x, R_{(n_i)}) = V^{s,u}(\bar x)\cap R_i.$ 

3)    $S( V^{s,u}(\bar x, R_{(n_i)}) = V^{s,u}(S\bar x, R_{S(n_i)})$. 

We call such a collection a {\bf Markov partition} of $\Delta$ for $F$.


Let $\Sigma_A^{\integer}=\otimes_{i \in \integer} \Sigma_A$   be  endowed 
  with the usual   product
topology ({\it Tykhonov topology}). For any $0< q<1, \bar \xi=(\xi_i), \bar
 \eta =(\eta_i) \in \Sigma_A^{\integer}$ define the distance $\rho_q(\bar 
\xi, \bar \eta)= sup_{i,j \in \integer} q^{|i| + |j|} |\xi_i(j) - \eta_i(j)|.$
 With the above  metric  compatible with its topology $\Sigma_A^{\integer}$ 
is a compact metric space. Let $\sigma^t $ and
$\sigma^s$  denote the two shift maps on $\Sigma_A^{\integer}$, i.e., 
 for $\bar \xi =(\xi_i) \in \Sigma_A^{\integer},$ $ \xi_i=\xi_i(j) \in 
\Sigma_A,$
$$(\sigma^t \bar \xi)_i(j) = \xi_i(j+1)\qquad \hbox{\rm \  and\ }\qquad
(\sigma^s \bar \xi)_i
= \xi_{i+1}.$$   We  define  the map $\bar \pi$: 
 $\Sigma_A^{\integer} \to \Delta = \otimes_{i} \Lambda$ by
$$\bar \pi : \bar \xi =(\xi_i) \to (\pi(\xi_i)), \quad \xi_i \in \Sigma_A.$$

The map $\bar \pi$ enables one to study   the uniqueness and ergodic properties
 of the equilibrium state for a  continuous function $\varphi$ on  $(\Delta,
\rho_q)$ by studying  the same properties  of the equilibrium state  for the
 corresponding   continuous function $\varphi \cdot \bar \pi$ on 
 $\Sigma_A^{\integer}$.  We introduce  now the concept of {\bf Gibbs states} 
for   H\"older continuous functions  on  $\Sigma_A^{\integer}$ and describe 
the relation between  Gibbs states and an equilibrium states.

 
Let $\varphi$ be a H\"older continuous function on $\Sigma_A^{\integer}$. Any
 element of $\Sigma_A^{\integer}$ is called a {\it configuration}. For any 
 subset $X \subset \integer^2 $, let
 $\Omega_X := \{ \xi_X | \hbox{\rm \  there \ exists }
\bar \xi \in \Sigma_A^{\integer} $   such that  $ \bar \xi|_X = \xi_X\}$
\ and  $X^C =  \integer^2 \setminus  X$. Elements of $\Omega_X$ are also 
called
the restriction of configurations to $X$.

For each finite subset $X \subset \integer^2 $, define the function 
$p_{\scriptscriptstyle X}(\bar \xi)$  on $\Sigma_A^{\integer}$
 by
$$ p_{\scriptscriptstyle X}(\bar \xi) = {  1
\over
\sum_{\bar \eta, \bar \eta|_{X^C} = \bar \xi |_{ X^C}} 
\exp(    \sum _{x \in \integer^2 } \varphi(\tau^x \bar \eta) - 
\varphi(\tau^x \bar \xi)) },$$ where $\tau^x$ denote the shift
$(\sigma^t)^i \cdot (\sigma^s)^j$ and   $x = (i,j)$.

{\bf Definition } [Ru]\qquad {\sl A probability measure $\mu$ on 
$\Sigma_A^{\integer}$
is called  a {\bf Gibbs state} for  $\varphi$ if for
any finite subset $X \subset \integer^2,$
$$ \mu_{\scriptscriptstyle X}(\xi_X) = \int_{\Omega_{X^C}} 
p_{\scriptscriptstyle X}(\bar \xi) d \mu_{\scriptscriptstyle X^C},$$
where $\mu_{\scriptscriptstyle X}$ and $\mu_{\scriptscriptstyle X^C}$ 
are the probability measures  on $\Omega_X$ and $\Omega_{X^C}$ that are
 induced by natural
projections  respectively.}

A transfer matrix $A$ is called  {\it aperiodic}   if there is a
positive integer $N$ such that every entry of the matrix $A^N$ is positive.

{\bf Proposition 2 }[Ru] \qquad {\sl If the transfer matrix $A$ is
 aperiodic, then $\mu$
is an  equilibrium state for $\varphi$ if and only if it is an invariant
 Gibbs state.}

Thus,  the   uniqueness and mixing property for  equilibrium
states becomes the problem of  the uniqueness and mixing property for 
 invariant Gibbs states provided that the function $\varphi$ is H\"older 
continuous. This problem has been extensively studied in statistical
mechanics in more general settings. It is  not true in general that for 
a H\"older continuous function the Gibbs state is unique. The  well-known
 Ising model  provides a class of counterexamples (see [MM]). The conjecture
 is that
uniqueness and mixing property hold for those functions defined in 
Theorem 7 (2). The potential functions constructed in [BS] and [PS] 
are of this type. The following proposition is a well-known result that
 is used to prove   Theorem 8 (2).    



{\bf Proposition 3 }  \qquad   [D] [Si] [MJ] {\sl Let $\Omega^{\integer^2}$
 be the fullshift on the lattice ${\integer}^2$, the invariant Gibbs
 state is unique for
any   H\"older continuous function on  $\Omega^{{\integer}^2}$ with a 
sufficiently small  H\"older constant. The Gibbs state is mixing with
 respect to  both horizontal and vertical shifts. }

  
 In this paper we obtain some partial results in this direction.  By
Theorem 4 the conjugating map $h$ between $(\Delta_{\Phi}, \rho_q)$ and 
$(\Delta, \rho_q)$ is H\"older continuous for some $0<q<1$. Since all 
metrics
$\rho_q, \ 0<q<1$ are H\"older equivalent, $h$ is actually H\"older
continuous for any $q$, \ $0<q<1$.  Thus  it suffices to 
consider the uniqueness of equilibrium states for H\"older continuous
 functions
on  $(\Delta, \rho_q)$ with respect to the $\integer^2-$action $\tau$
 induced by $(F,S)$. We denote the $\integer^2-$action on $\Sigma_A^{\integer}$
 by $\tau^*$.

{\bf Lemma 6.1}\qquad {\sl  The semiconjugacy $\bar \pi $ between $\Delta$ and
 $\Sigma_A^{\integer}$  has the following properties:

1) $\bar \pi$ is surjective and H\"older  continuous from $\Sigma_A^{\integer}$
  to $(\Delta, \rho_q)$ for any $0<q<1$  (it is actually Lipschitz continuous).

2)
 $$\bar \pi \cdot \sigma^t = F \cdot \bar \pi ,\qquad
\bar \pi \cdot \sigma^s = S \cdot \bar \pi,\ \hbox{\rm i. e., }\ \bar\pi
 \cdot \tau^* = \tau \cdot \bar \pi, $$
where $\sigma^t$ and $\sigma^s $ are two shift maps on $\Sigma_A^{\integer}$.

3)  $\bar \pi$ is injective outside the set $ \bar \pi ^{-1}(\BB)$, where
 $\BB$ denotes the boundary of the Markov partition of $\Delta$.

}



{\bf Lemma 6.2}  \qquad {\sl 
1)  Let $\varphi$ be a H\"older continuous function on $\Delta$ and
 let $\varphi^* = \varphi \cdot \bar \pi$. Then $P_{\tau^*}(\varphi^*)
 \geq P_{\tau}(\varphi).$

2)  Assume that $\mu^*$ is a $\tau^*$ invariant measure on 
$\Sigma_A^{\integer}$ and  measure $\mu$ on $\Delta$ satisfies  
 $\mu (E) = \mu^* ({\bar \pi}^{-1}(E))$ for any Borel set $E$ of $\Delta$.
 Then  $ h_{\tau}(\mu) \leq h_{\tau}(\mu^*).$  Furthermore, if 
 $\mu^*({\bar \pi}^{-1}(\BB))=0$   then,  $ h_{\tau}(\mu) = h_{\tau}(\mu^*)$. 
}




{\bf Theorem 6} \qquad {\sl
Let $\varphi$ be H\"older continuous on $\Delta$. Assume that 
 $\mu^*({\bar \pi}^{-1}(\BB))=0$  for any equilibrium
states $\mu^*$ for $\varphi^* = \varphi \cdot \bar\pi$. Then,

1)  
the measure $\mu$ defined by $\mu (E) = \mu^* ({\bar \pi}^{-1}(E))$
is an equilibrium state on $\Delta$ for $\varphi$ and  $P_{\tau^*}
(\varphi^*) = P_{\tau}(\varphi);$



2)  if $\mu $ is an equilibrium state  on $\Delta$ for   $\varphi$
then there exists an equilibrium state $\mu^*$ for $\varphi^*= 
\varphi \cdot \bar \pi$ on
$\Sigma_A^{\integer}$ with the property $\mu (E) = \mu^* ({\bar \pi}^{-1}(E))$
 for any Borel set $E \subset \Delta$.
}

 



{\bf Theorem 7 } \qquad {\sl
 1)  Assume $\mu^*$  is an equilibrium state  ergodic with respect to
 the vertical shift
$\sigma^t$ for a H\"older continuous function
on  $\Sigma_A^{\integer}$. Then  $\mu^*({\bar \pi}^{-1}(\BB))=0$.


 
 2) For any $0 < q < 1, 0 < \alpha <1 ,$ and  any aperiodic matrix $A$
 there exists a small constant $c$ such that if  $\psi$ is a H\"older
 continuous function on $\Sigma_A^{\integer}$ satisfying the following 
condition
 $$  |\psi( \bar \xi ) - \psi(\bar \eta )| \leq c \rho_q^{\alpha}
(\bar \xi, \bar \eta) $$ for any $\bar \xi = (\xi_i), \bar \eta =(\eta_i) 
\in \Sigma_A^{\integer}$ with $ \xi_0 = \eta_0$, then  $\mu^*({\bar \pi}^{-1}
(\BB))=0$ holds for any equilibrium state
$\mu^*$ for $\psi$.

 }
 

{\bf Corollary} \qquad {\sl Let $\varphi$ be   a H\"older continuous 
function   on $\Delta$ satisfying the condition  
$$  |\varphi(\bar x) - \varphi(\bar y)|
\leq c \rho_q^{\alpha}(\bar x , \bar y ), $$ where $\bar x = (x_i), 
\bar y=(y_i) \in \Delta , x_0 = y_0 $, and $c$ is sufficiently small. 
Then the equilibrium state for $\varphi$ is unique if and only if the
 equilibrium state   for $\varphi^*= \varphi\cdot\bar\pi$ is unique on
 $\Sigma_A^{\integer}$.}


   

{\bf Theorem 8} \qquad {\sl 
1)   There is a unique  measure $\mu$ on $\Delta_{\Phi}$ such that the 
entropy $h_{\tau}(\mu)$ attains its supremum and this measure of maximum 
entropy is mixing and  positive on open sets. 

2) Assume that  the
symbolic presentation for $(\Phi, S)$ is given by the fullshift on
$\integer^2$
 ( e.g. $\Lambda$ is a Smale horseshoe).  
   If $\varphi$ is a   H\"older continuous function with a sufficiently
 small H\"older constant on $(\Delta_{\Phi}, \rho_q)$, 
then the equilibrium state for $\varphi$ is unique, mixing with respect
 to $\tau$ and positive on open sets.  
}
 



\vskip1cm





      %%%%%%%%%%%%%% PROOFS START HERE%%%%%%%%%%%%%%%%%%%%%%%%%%








                \centerline{ \bf 4. PROOFS}


{\bf Proof of Theorem 1}\qquad The first statement of the theorem follows
 from the classic   graph transform technique. The proof of  the second
statement   is a modification of   the proof  in the finite dimensional case  
[KH] [Sh] and is an immediate consequence of the following shadowing lemma:

{\smalltype \bf Shadowing Lemma}\quad{\it There exist a neighborhood 
$U(\Delta) \supset \Delta
$ and $\eps_0, \delta_0 >0$ such that for all $\delta >0,$ there is an 
$\eps >0$ with the following property:\hb
If $\Phi=F \cdot G : U(\Delta) \to \MM$, is a diffeomorphism with $G$
 $\eps_0$-close
to $id$\  in the $C^1$-topology, $Y \subset U(\Delta)$, is a subset and
$Q: \ Y \to Y$, a homeomorphism with  
$$  \dist_{C^0}(Q, \Phi) = \sup_{y \in Y}(Q(y), \Phi(y)) \leq \eps,$$
then, there exists a unique $h \in C^0(Y, U(\Delta))$ such that
$h \cdot Q = \Phi \cdot h$   with $ \dist_{C^0}(h, id) < \delta$. 
}


{\it Proof} \qquad   Define a map $$\FF :  C^0(Y, U(\Delta)) \to C^0(Y, \MM)
\eqno(1.1)$$
 by $ \beta \longmapsto \Phi \cdot \beta \cdot Q^{-1}.$ For $y \in Y$, 
$\FF \beta(y)= \Phi\cdot \beta (Q^{-1}(y))$.           We wish to show 
that $\FF$ has a unique fixed point near the identity.

Set
$$C^0_s(Y, T\MM) = \{ v \in C^0(Y, T\MM) \ : \ v(y) \in T_{\bar y}\MM,
 y \in Y\}.$$ We denote by $\cal I$ the identity embedding of $Y$ into $\MM$ . 
Let   $B_{\gamma}(\cal I)$ be  the ball in $ C^0(Y, U(\Delta))$ centered 
at $\cal I$ with radius $\gamma$. Consider the map $\AA: B_{\gamma}(\cal I)
 \to C^0_s (Y, T\MM)$ defined by
$$\AA \beta(\bar y) = (\exp^{-1}_{y_i} \beta_i(\bar y) )_{i \in \integer}.
\eqno(1.2)$$
The map  $\AA$ is well-defined when $\gamma$ is small and is a homeomorphism
 onto $B_{\gamma}(0) \subset
C^0_s(Y, T\MM)$, where  $B_{\gamma}(0)$ is the ball centered at the zero 
section $0$ with radius $\gamma$.

Define $$ \FF' = \AA \cdot \FF \cdot \AA^{-1}: \  B_{\gamma}(0) \to 
C^0_s(Y, T\MM).\eqno(1.3)$$  If $v \in  B_{\gamma}(0) $ is a fixed point 
of $\FF'$, then
$\AA \cdot \FF \cdot \AA^{-1} v =v$. Hence, the preimage of $v$, $\AA^{-1}v 
\in B_{\gamma}(\II)$, is a fixed
point of $\FF$ and the proof is then completed.

To show that $\FF'$ has a fixed point in $B_{\gamma}(0)$,   we note that 
$ C^0_s(Y, T\MM)$ is a Banach space and the map $\FF'$ is  differentiable
 in $ B_{\gamma}(0) $. In fact, $D\FF'$ is Lipschitz in $v$ since
the exponential map and its inverse are smooth. 
By the hyperbolicity of $F$,  without making any major changes we can
 similarly claim the following  (Lemma 18.1.4 in [KH]).

{\it Claim \quad }{\it There exist a neighborhood $U(\Delta) \supset \Delta, 
\eps_0, \eps >0$, and $R >0$ independent of $Y, Q$, so that 
$$\|(D\FF')|_0 - Id )^{-1}\| <R, \ \hbox{\it where}\ \dist_{C^1}(F, F') 
< \eps_0,
\dist_{C^0}(Q, F') < \eps.$$  }

Then, we define a map $ \KK:  B_{\gamma}(0) \to  C^0_I(Y, T\MM)$ by 
$$\KK v = -( (D\FF')|_0 - Id)^{-1} \cdot \HH v,\eqno(1.4)$$ where 
$\HH v =\FF' v - (D\FF')|_0 v$.  By  estimating the Lipschitz constant
 of $\KK$ near $0$ and $\| \KK(0)\|$, we can see that if $\eps_0, \eps$
 are chosen
small enough, the mapping $\KK$ is a contraction in a smaller ball
$ B_{\gamma_0}(0) \subset  B_{\gamma}(0) \subset  C^0_s(Y, T\MM)$ and
 $\KK(B_{\gamma_0}(0)) \subset B_{\gamma_0}(0)$. Thus it has a unique 
fixed point in
$ B_{\gamma_0}(0) $. Obviously, $v$ is also a fixed point of $\FF'$. 
This finishes the proof of the shadowing lemma.


 





{\bf Proof of Theorem 2}\qquad Since $(\Delta, F)$ and $(\Delta_{\Phi}, \Phi)$
 are topologically conjugate we need only to prove the theorem for  
$(\Delta, F)$.  By assumption  $f|_{\Lambda}$ is topologically mixing 
and $\Lambda$ is locally maximal. One can directly see that
$\Delta$ is locally maximal. To show that $F|_{\Delta}$ is topologically
 mixing, it suffices to show that the global unstable manifold of any 
periodic point 
 $\bar x \in \Delta$ is dense in $\Delta$ and that the periodic points 
of $F$ are dense in $\Delta$. 

Let $\bar x = (x_i)$ be a periodic point of $F$ and let $W^u(x_i)$ denote
 the global unstable manifold for $f$ at  the point $x_i \in M_i$. Then
 $\bigotimes W^u(x_i)$ is the global unstable manifold for $F$ at the
 point $\bar x = (x_i)$,  which is clearly dense in $\Delta$ since 
$W^u(x_i)$ is dense in $\Lambda$.

Since $f|_{\Lambda}$ is hyperbolic and topologically mixing, the 
periodic points of $f$ are dense in $\Lambda$. By the   compactness 
of $\Lambda$, one can further see that for
any $\eps >0$, there exists an integer $N(\eps)> 0$ 
such that in the $\eps$-neighborhood of  any $x \in \Lambda$, there 
is a periodic point with a prime period less than $N(\eps)$.

To show that periodic points of $F$ are dense in $\Delta$, let us
 take a point
$\bar x= (x_i) \in \Delta$ and its $\eps$-neighborhood $B_{\eps}
(\bar x)  =\bigotimes B_{\eps}(x_i)$. Pick a periodic point $z_i$
in $B_{\eps}(x_i)$ with the prime
period less that $N(\eps)$ for each $i$. Then, $\bar z = (z_i)$ is 
a periodic point of $F$ 
in $B_{\eps}(\bar x)$. Its prime period is less than   $N(\eps)!$.

















{\bf Proof of Lemma 1} \qquad We first fix $i \in \integer$ and let
  $\bar x, \bar y \in \MM $ with $x_j = y_j, j\not= k$ and  $0 <\theta< q <1$.
If  $i\not=k  \in \integer$, then
$$ q^{|i|} d(G_i(\bar x), G_i(\bar y) ) =  q^{|i|} d(G_0(S^i \bar x), 
G_0(S^i \bar y) ) \leq C  q^{|i|} \theta ^{|k -i|} d(x_k, y_k)$$ 

$$\leq C q^{|i|} q^{|k -i|} ( {\theta \over q})^{|k -i|} d(x_k, y_k)
\leq C q^{|k|}( {\theta \over q})^{|k -i|} d(x_k, y_k).$$
 If $i = k$, then
$$ q^{|i|} d(G_i(\bar x), G_i(\bar y) )  \leq C q^{|k|} d(x_k, y_k).$$
Thus, for every fixed $i$ and  arbitrary $\bar x, \bar y \in \MM$, we
 have
$$q^{|i|} d(G_i(\bar x), G_i(\bar y) ) \leq C ( 1 +\sum_{k\not= i}
( {\theta \over q})^{|k -i|} ) \sup_{n \in \integer} q^{|n|}d(x_n, y_n)$$
$$
=C (1  + {2\theta \over q -\theta}) \sup_{n \in \integer} q^{|n|}d(x_n, 
y_n).$$
Therefore, we have  $ \rho_q(G(\bar x), G(\bar y)) \leq C(1+{2\theta 
\over q -\theta}) \rho_q(\bar x, \bar y)$. 

 The proof of the second part of the lemma is trivial.
As an easy corollary of Lemma 1 one can see that if both $G, G'$ are  
  short ranged, then the composition $G \cdot G'$ is also  short ranged.







{\bf Proof of Lemma 2} \qquad 
 $(1) \Rightarrow (2)$: \ Without loss of generality we assume $G$ is
 a $C^1$ diffeomorphism of $\MM$. The tangent space $T_{\bar x}\MM $ at
 any point $\bar x = (x_i)$ is a product space $\bigoplus T_{x_i}M_i$ 
which is equipped with a Finsler metric. We write $G$ in the coordinate form:
$G = ( \cdots G_{-n}, \cdots, G_{-1}, G_0, G_1, \cdots, G_n, \cdots)$. Then
the differential $DG $ can be expressed as  
$$DG=  ( \cdots DG_{-n}, \cdots, DG_{-1}, DG_0, DG_1, \cdots, DG_n, \cdots).
$$
Without loss of generality, let us consider
the linear mapping $DG_0: \bigoplus T_{x_i}M_i \to T_{y_0}M,$ where
$(\bar y)=(y_i)=G(\bar x) $. Let  $\bar \xi= (\xi_i) \in 
\bigoplus T_{x_i}M_i $ be  any tangent vector satisfying $\xi_i =0 $ 
except $i=k$ for some fixed $k \in \integer.$  Consider a smooth curve 
$\gamma(t)$ in $M_k$ passing
through $x_k$ with ${d \gamma(t)\over dt}|_{t=0}= \xi_k$. Then 
$\Gamma(t): t \to
( \cdots, x_{k-1}, \gamma(t), x_{k+1}, \cdots)$ \  is a smooth curve
 in $\MM$ passing through $\bar x$ with ${d \Gamma(t)\over dt}|_{t=0}=
 \bar \xi$. Thus 
$$\| D_{\bar x}G_0(\bar \xi) \|= \| d G_0(\Gamma(t))/dt \|
= \lim_{t \to 0} {\| G_0(\Gamma(t)) - G_0(\bar x)\|\over |t|}$$ 
$$\leq C \theta^{|k|} \lim_{t \to 0} {\|\gamma(t) - x_k\|\over |t|} =
 C \theta^{|k|} \|\xi_k\|.$$

$(2) \Rightarrow (1)$: For  any integer $k \in \integer$ and  two points
 $\bar x=(x_i), \bar y=(y_i) \in \MM $ with $x_i = y_i$ for $i \not= k$, 
let $\Gamma(t)$ be a geodesic connecting $x_k$ and $y_k$ in the compact 
manifold $M_k=M$, $t \in  [0,l]$. $\alpha: t \to ( \cdots, x_i,\cdots,
 x_{k-1},
 \Gamma(t), x_{k+1},\cdots)$ defines a smooth curve from $[0,l]$ to $\MM$. 
$d(G_0(\bar x), G_0(\bar y))$ 
$$= d (G_0(\alpha(0)), G_0(\alpha(1))) \leq  \max_t \{\|DG_0|_{\alpha(t)}
\xi_k\|  \cdot \|D\Gamma(t)\|\} d( x_k,  y_k),\eqno(2.1)$$
where $\xi_k$ is a unit tangent vector in $T\MM$ with every coordinate zero
except the $kth$. By assumption,  $\|DG_0|_{\alpha(t)}\xi_k\| \leq C 
\theta^{|k|}$. Then the inequality (2.1) means that $G$ is short ranged 
with a decay constant $\theta$.

 $(1) + (2) \Leftrightarrow (3)$ is  obvious.








{\bf Proof of Lemma 3}\qquad
By Lemma 2, the properties of  linear short range mappings can then
  be passed on
to those differentiable mappings between Banach manifolds.  Let 
$l^{\integer}$ be the Banach space  $$\{ x= (x_i)\  : \quad x_i \in 
\real^m,  i \in \integer, \sup_{i \in \integer} \| x_i\| < \infty \} 
\eqno(3.1)$$ with the norm   $\|x\| = (x_i)\ $ is $ \sup_{i \in \integer}
 \| x_i\| $. Any linear operator $A$ of $l^{\integer}$
can be expressed as an infinite matrix in the usual  weak* basis: 
$A=(a_{ij}); -\infty < i,j < \infty$, where $a_{ij}$ are linear operators
 of $\real^m $. The operator  $A$ is said to be shift invariant if 
$a_{i j} = a_{i+1 j+1}; -\infty < i,j < \infty$ and $A$ is said to be short
ranged if $\| a_{i j}\| \le C \theta^{|i-j|}$ for some constant $C>0$ and 
$0 <\theta < 1$. To prove Lemma 3, we need only to show the following 
statement.


 {\it Claim}\quad {\it Let $A$ be an invertible linear operator on 
$l^{\integer}$ and $I$ the identity. For any $C> 0, $ and $0< \theta<\theta'<1$ 
there exists $\eps >0$ such that if $A$ is a   short
range operator with constants $C$ and $\theta$ and $\| A - I\| \leq \eps$,
 then the inverse $A^{-1}$ is also a short ranged mapping with the decay 
constant $\theta' $. }




{\it  Proof} \qquad  For convenience we prove the claim when $m=1$. Let us 
first express the operator $A$ in a form of an infinite matrix $(a_{ij})$
 under the usual $\hbox{\rm weak}^*$ basis. Then  $A$  has the short range
 property if and only if $|a_{ij}| \leq C \theta^{|i-j|}$, where $\theta $ 
is the decay constant and $C$ is the other constant in the definition
of  short range mappings. It is easy to see that such an infinite matrix
also defines a bounded linear operator of the   Banach space:
$$l_{\theta '}^{\integer}= \{ x=(x_i) \ : \  x_i \in \real, i \in \integer,
 \sup_{i \in \integer} (\theta')^{|i|}|x_i| < \infty\}$$ endowed with the
 norm   $\|x\|_{\theta'}= \sup_{i \in \integer} (\theta')^{|i|}|x_i|$.   
 We estimate the norm
of $I - A$ in the  Banach space $l_{\theta '}^{\integer}$. 
$$ \|(I -A)(x_j)\|_{\theta'} = 
\sup_{i \in \integer} (\theta')^{|i|} |(1-a_{ii})x_i + \sum_{j \not= i} 
a_{ij} x_j |$$
$$ \leq \sup_{i \in \integer}  (\theta')^{|i|}  (|(1-a_{ii})x_i | 
+ \sum_{j \not= i}| c_{ij} |\theta^{|i-j|} |x_j|),\eqno(3.2)$$ 
where $c_{ij} \theta^{|i-j|} = a_{ij}$ and $|c_{ij}| \leq C$. 
Thus,
$$  \|(I -A)(x_j)\|_{\theta'} \leq \sup_{i \in \integer}  (|(1-a_{ii})| 
 {\theta'}^{|i|} |x_i |
+  \sum_{j \not= i} | c_{ij} |{\theta^{|i-j|} \over (\theta')^{|j|-|i|}} 
(\theta')^{|j|}  |x_j|)$$
$$ \leq \sup_{j \in \integer} (\theta')^{|j|}  |x_j| \ 
 \sup_{i \in \integer} ( | 1- a_{ii}| +  \sum_{j \not= i} | c_{ij}| 
{\theta^{|i-j|} \over (\theta')^{|j|-|i|}} ).$$
Obviously, $|1-a_{ii}| \leq \eps $ when $\| A -I\| \leq \eps$. Note 
that $${\theta^{|i-j|} \over (\theta')^{|j|-|i|}} \leq  ({\theta \over 
\theta'})^{|i-j|}$$
 and $\sum_{j \not= i}| c_{ij} |\theta^{|i-j|} \leq \eps$.  Let us choose 
an integer $K >0$ such that \hb
$ 2C \sum_{n=K+1}^{\infty} ({\theta \over \theta'})^n \leq 1/4$
 and   $ 0< \eps < (1/4) \theta^K$. Then, 
$$  \sum_{0<|i-j |\leq K} | c_{ij}| {\theta^{|i-j|} \over (\theta')^{|j|-|i|}}
       \leq \eps/ (\theta')^K < (1/4).$$ 
 Therefore,  $$\sup_{i \in \integer} ( | 1- a_{ii}| +  \sum_{j \not= i}
 | c_{ij}| {\theta^{|i-j|} \over (\theta')^{|j|-|i|}}   ) < \eps + 1/4 +
 1/4 <1.$$
Thus   $ \|(I -A)\|_{\theta'} <1$,  which implies that $A$ is invertible
 on $l_{\theta '}^{\integer}$. It is easy
to see that the boundedness of $A^{-1}$ on  $l_{\theta '}^{\integer}$
 implies
that $A^{-1}$ is a short range mapping on $l^{\integer}$ with the decay
 constant
$\theta'$. If we denote the entries of the infinite matrix representing
 $A^{-1}$ by $b_{ij}$, then there exists a constant $C'$ such that 
$|b_{ij}| \leq C' ( \theta')^{|i-j|}$. One can also see that the constant 
$C'$ depends only on constants
$C, \theta,$ and $\theta'$.


{\bf Remark.} \quad As an easy corollary of Lemma 3, one can show 
that if $F$ and $F^{-1}$ are both short ranged diffeomorphisms of
 $\MM$ and  the $C^1$ distance between $F$ and $G$ is sufficiently
 small, then
 $G^{-1}$ is also short ranged.







{\bf Proof of Lemma 4}\qquad  
For any $|i-k| \geq k_0, k_0 \in \natural $  fixed, $0 < q <1$, and 
$\bar x, \bar y $ with $x_j = y_j, j\not= k$, 
$$ q^{|i|} d(G_i(\bar x), G_i(\bar y) ) =  q^{|i|} d(G_0(S^i \bar x),
 G_0(S^i \bar y) ) \leq C q^{|i|} \theta ^{|k -i|} d(x_k, y_k)$$ 

$$\leq C q^{|i|} q^{|k -i|} ( {\theta \over q})^{|k -i|} d(x_k, y_k)
\leq C q^{|k|}( {\theta \over q})^{|k -i|} d(x_k, y_k).$$
For $i=k, $
$$ q^{|i|} d(G_i(\bar x), G_i(\bar y) ) =  q^{|i|} d(G_0(S^i \bar x),
 G_0(S^i \bar y) ) \leq  q^{|k|} (1 + \delta)d(x_k, y_k)$$
For $0 < |i - k| < k_0 $,
$$ q^{|i|} d(G_i(\bar x), G_i(\bar y) ) =  q^{|i|} d(G_0(S^i \bar x),
 G_0(S^i \bar y) ) \leq  q^{|i|} \delta d(x_k, y_k)$$
$$ = q^{|i| - |k|} \delta q^{|k|} d(x_k, y_k) \leq  q^ { -|i-k|} \delta
 q^{|k|} d(x_k, y_k).$$
Therefore,  for every fixed $i \in \integer$ and for arbitrary $\bar x,
 \bar y \in \MM$, we have 
$$q^{|i|} d(G_i(\bar x), G_i(\bar y) ) \leq ( 1+ \delta (\sum_{l=0}^{k_0-1}
 q^{-l})      +   \sum_{|k- i| \geq k_0}
( {\theta \over q})^{|k -i|} ) \sup_{i \in \integer} q^{|i|}d(x_i, y_i)$$
$$= [1 + \delta (q^{-k_0} -1)(q^{-1}-1 )^{-1}  + 2({\theta \over q })^{k_0} 
({q \over q -\theta})] \sup_{i \in \integer} q^{|i|}d(x_i, y_i).$$
We first fix $k_0$ so that $$2({\theta \over q })^{k_0} 
{q \over q -\theta} \leq \eps/2,$$ and then choose  $\delta$   so that
 $$\delta  (q^{-k_0} -1)(q^{-1}-1 )^{-1} \leq \eps/2.$$  Thus, we have 
$ \rho_q(G(\bar x), G(\bar y)) \leq (1+ \eps)\rho_q(\bar x, \bar y).$
By the virtue of Lemma 3 one can further show that  $\delta$ can
be chosen so small that the inverse $G^{-1}$ is also Lipschitz continuous 
in the metric $\rho_q$ with
a Lipschitz constant less than $1 + \eps$.






{\bf Proof of Theorem 3}\qquad  We prove a  modified  version of the
 shadowing lemma.




{\smalltype \bf Modified  Shadowing lemma}\quad {\it There exist a
 neighborhood $U(\Delta) \supset \Delta
$ and $\eps_0, \delta_0 >0$ such that for all $\delta >0,$ there is 
an $\eps >0$ with the following property:\hb
If $\Phi=F \cdot G : U(\Delta) \to \MM$, is a short ranged diffeomorphism 
with $G$ $\eps_0$-close
to $id$ in the $C^1$-topology, $Y \subset U(\Delta)$, is an subset and
 $Q: \
Y \to Y$, a homeomorphism with both $Q$ and $Q^{-1}$  short
ranged and 
$$  \dist_{C^0}(Q, \Phi) = \sup_{y \in Y}(Q(y), \Phi(y)) \leq \eps,$$
then, there exists a unique $h \in C^0(Y, U(\Delta))$ such that
$h \cdot Q = \Phi \cdot h$   with $ \dist_{C^0}(h, id) < \delta$. The
 map $h$ is also  continuous in the metric $\rho_q$.}






{\it Proof} \qquad Following the the proof of the shadowing lemma and 
using lemmas 1 - 3,  one  can easily   check that
the short range property is preserved at all steps of  this  proof.


To complete the proof of Theorem 3,
 let us first choose $Y=\Delta$, $Q=F$. By applying the modified shadowing
theorem we obtain a mapping $h: \Delta \to U(\Delta),$  satisfying
 $h \cdot F = \Phi \cdot h$.
$h$ is  $\rho_q$ continuous. $\Delta_{\Phi}=h(\Delta)$ is invariant
under $\Phi$.
Then, we choose $Y= h(\Delta)$, $Q=\Phi$, and $\Phi=F$ in   the modified
 shadowing lemma. Since $\dist_{C^1}(\Phi, F) < \eps_0$, Lemma 3  
indicates that $\Phi^{-1}$ is
also short ranged. Thus, there exists $\beta$ such that $ \beta \cdot 
\Phi =
F \cdot \beta$. Finally, when we choose $Q=F$ and $\Phi=F$, we have 
$$(\beta \cdot h )\cdot F = \beta \cdot \Phi \cdot h = F \cdot 
(\beta \cdot h).$$
By the uniqueness, we conclude that $\beta \cdot h =id$. Thus, both
 $h,      h^{-1}(=\beta)$ are continuous in the metric $\rho_q$.










{\bf Proof of Theorem 4} \qquad 
The proof is divided into three major steps.

{\it Step 1 } \qquad  We first prove that   H\"older continuity
for the conjugacy $h$ follows from the following statement:

{\it There exist constants $C >0, \delta_1 >0$, and $ 0 < \alpha <1 $
 such that
for any $ \bar y \in V^u(\bar x) \cap \Delta$ or $ \bar y \in V^s(\bar x)
\cap \Delta$ with $ \rho(\bar x, \bar y) \leq \delta_1$
$$ \rho_q(h(\bar x), h(\bar y)) \leq C \cdot \rho^{\alpha}_q(\bar x, \bar y),
\eqno(4.1)$$
where $V^s(\bar x),V^u(\bar x)$
 are the local stable and unstable manifolds at $\bar x$ respectively.}


In fact, since $\Delta$ is locally maximal, it has a local product structure,
i.e., there exists 
$\delta_0  >0$ such that  for any two points $\bar x, \bar y \in \Delta $
with $ \rho(\bar x, \bar y) < \delta_0$, $V^s(\bar x) \cap V^u(\bar y)$
consists of a single point $\bar z=[\bar x,\bar y]$  and $ \bar x \in
 V^s(\bar z), \bar y \in V^u(\bar z)$. Now, let us assume that the previous
statement is true. We can choose $\delta_0$ sufficiently small so that
$\rho(\bar x, \bar z) < \delta_1$ and $\rho(\bar y, \bar z) < \delta_1$
whenever $\rho(\bar x, \bar y) < \delta_0$. Thus, 
$$ \rho_q(h(\bar z), h(\bar x)) \leq C \rho_q^{\alpha}(\bar z, \bar x), 
\quad
\rho_q(h(\bar z), h(\bar y)) \leq C \rho_q^{\alpha}(\bar z, \bar y).$$
Hence, for any $\bar x, \bar y \in \Delta$ with $\rho(\bar x, \bar y) <
 \delta_0$, we have
$$\rho_q(h(\bar x), h(\bar y)) \leq C [\rho_q^{\alpha}(\bar z, \bar x) +
\rho_q^{\alpha}(\bar z, \bar y)]$$
$$= C \{[ \sup_i q^{|i|} d(x_i, z_i)]^{\alpha} + 
[ \sup_i q^{|i|} d(y_i, z_i)]^{\alpha}\}$$
$$ \leq C' [ \sup_i q^{|i|} d(x_i, y_i)]^{\alpha}= C' \rho_q^{\alpha}
(\bar x, \bar y).$$ The last inequality holds because
stable and unstable manifolds are   transversal uniformly over $i \in 
\integer$
and $x_i, y_i$.


Now let us consider the H\"older continuity along the global stable 
and unstable
manifolds. Let $d'$  be the induced metric on the global  stable
 manifold   $W^s(x)$  at any point $x \in \Lambda$. Let $l$ be a 
fixed positive number. For
any $y \in W^s(x)$ with $d'(x,y) < l$, there exists a positive 
integer $N(l)$ which solely depends on $l$ and $\lambda$ such that 
$d(f^{N(l)}(x), f^{N(l)}(y))
\leq \delta_0$. Then,
$$\rho_q(h(\bar x), h(\bar y)) = \rho_q(hF^{-N(l)}F^{N(l)}(\bar x), h 
 F^{-N(l)}F^{N(l)}(\bar y) )$$
$$
= \rho_q(\Phi^{-N(l)}h F^{N(l)}(\bar x), \Phi^{-N(l)}h F^{N(l)}(\bar y) )
\leq  L^{N(l)} \rho( h F^{N(l)}(\bar x), h F^{N(l)}(\bar y) )$$
$$\leq C L^{N(l)}  \rho_q^{\alpha}(\bar x, \bar y),$$ where $L$ is the
 Lipschitz
constant of $\Phi^{-1}$ in the  metric   $\rho$. Along  the global 
unstable manifolds, we have a similar estimation.


In general,   by the compactness
and the topological mixing property  of $\Lambda$ there exists $l \geq 0$
 such that for arbitrary two points $\bar x, \bar y \in \Delta$,, one 
 can find a fixed integer $k \in \natural$ 
and a sequence of points  $\bar x_0 =\bar x, \bar x_1, \cdots, \bar x_k =
 \bar y \in \Delta$
with the following properties: 

1) $\bar x_{2n+1} \in W^u(\bar x_{2n}), n =0, 1,2,\cdots$ and
 $ \bar x_{2n} \in W^s(\bar x_{2n-1}), n=1,2,\cdots.$

2)  $d'((\bar x_n)_i, (\bar x_{n+1})_i) < l,  \ n=0,1, \cdots, k-1;
 \ i \in \integer .$

Thus,
 $$\rho (h(\bar x), h(\bar y) \leq \sum_n  \rho_q^{\alpha}( h(\bar x_n),
h(\bar x_{n+1}))$$
$$ \leq C'' \sum_n \rho_q^{\alpha}(\bar x_n, \bar x_{n+1}) \leq kC''
\rho_q^{\alpha}(\bar x, \bar y).$$  This proves the H\"older continuity 
of   the conjugacy $h$    in the  metric
$\rho_q$ when  the statement is assumed   true.

 To prove the statement itself, we  need only to show that it is true when
$\bar y \in V^u(\bar x)$ by the symmetry.  One can easily prove the H\"older
continuity of the conjugacy $h$ in the Finsler metric by applying the
 usual technique
 [KH]. However, this kind of technique fails when we deal with the
 metric $\rho_q$.
We shall  show that $h$
satisfies  $(4.1)$ by examining the procedure in which the map $h$
 is constructed.


Let $\bar x \in \Delta$. Then $h(\bar x) \in \Delta_{\Phi}$   is hyperbolic
for $\Phi$ and there exist the local stable and unstable manifolds
$V^s_{\Phi}(h(\bar x)), V^u_{\Phi}(h(\bar x))$ passing through $h(\bar x)$.
For any $\bar y \in V^u(\bar x)\cap \Delta$ with $\rho(\bar x, \bar y) <
 \delta_1$, $h(\bar y) \in  V^u_{\Phi}(h(\bar x)) \cap \Delta_{\Phi}$.
Note that $h(\bar y)$ is exactly the unique intersecting point of 
$V^s_{\Phi}(h(\bar y))$ and $ V^u_{\Phi}(h(\bar x))$. By the short range 
property of the perturbation and the transversality of the stable and
unstable manifolds, we see that if one can show the unstable manifold
$V^s_{\Phi}(h(\bar y))$ varies H\"older continuously in the  metric
 $\rho_q$ with
respect to $\bar y$, then the H\"older continuity of $h$ in the 
 metric $\rho_q$ follows. 

{\it Step 2} \qquad  
We consider the exponential splitting of the tangent bundle at $\bar x$
 under map $F$:
$$T_{\bar x} \MM  = E^u_{\bar x} \oplus E^s_{\bar x}, \ n=0,1,2, \cdots.
  \qquad  DF E^u_{\bar x} = E^u_{F(\bar x)}; \  DF E^s_{\bar x} = 
E^s_{F(\bar x)}.$$
Let $B_{\gamma} ( \bar x)$ denote the $\gamma$-ball in
 $T_{  \bar x}\MM$ centered at $\bar x$ and  
$\  B^u_{\gamma}( \bar x) = B_{\gamma} ( \bar x) \cap E^u_{\bar x} 
\quad B^s_{\gamma} ( \bar x ) = B_{\gamma} (\bar x) \cap E^s_{\bar x}.$
When $\gamma$ is   small and $\Phi $ is sufficiently  close to $F$ 
 the following
map  
$$\FF_{\bar x} : B_{\gamma} ( \bar x) \to T_{ F (\bar x)}\MM,\ 
 n =1,2,\cdots$$
$$\FF_{\bar x} \bar \xi = \exp^{-1}_{F (\bar x)} \cdot \Phi \cdot 
\exp_{ \bar x}( \bar \xi)$$  is well defined.
Now let us consider  the $C^1-$manifold   ${\widetilde V}^s_{\Phi}
(h(\bar x))= \exp^{-1}_{ \bar x} V_{\Phi}^s(h(\bar x))$ in $B_{\gamma}
( \bar x)$.   
  Since  $\dist_{C^0}(h,id)$ is small, the manifold
${\widetilde V}^s_{\Phi}(h(\bar x))$ can be obtained  by applying the 
graph transform technique. Namely, we consider maps
$$ \varphi_{\bar x}(t): B^s_{\gamma}( \bar x) \to B^u_{\gamma}( \bar x), \ 
n=0,1,\cdots$$
 such that 
$$ \{ (t, \varphi_{\bar x}(t)) :  t \in B^s_{\gamma}( \bar x) \} = 
{\widetilde V}^u_{\Phi}(h(\bar x))$$
 is invariant under map $\FF_{\bar x}$.
For any $\bar \xi = (u, v) \in B_{\gamma}(\bar x) \subset B^s_{\gamma}
( \bar x) \oplus B^u_{\gamma}(\bar x),$ the map $\FF_{\bar x}$ can be
written as 
$$\FF_{\bar x} \cdot \pmatrix{u \cr 
                     v \cr}= D\FF_{\bar x}  \cdot \pmatrix{u \cr 
                     v \cr} + \pmatrix{g_{1,\bar x}(u,v) \cr  g_{2, \bar x}
(u,v) \cr},$$
   By the hyperbolicity of $\Phi$, the differential  $D\FF_{\bar x} = 
D\exp_{F(\bar x)}^{-1} D\Phi D\exp_{\bar x}$ can be  written as follows.  
$$D\FF_{\bar x} =\pmatrix{P_{11}(\bar x) & P_{12}(\bar x)\cr
                P_{21}(\bar x) & P_{22}(\bar x)\cr }$$ 
where $ P_{11}(\bar x): E^s_{\bar x} \to  E^s_{F(\bar x)},  P_{21}(\bar x):
 E^s_{\bar x} \to  E^u_{F(\bar x)}, P_{12}(\bar y): E^u_{\bar x} \to 
 E^s_{F(\bar x)}, $ and $ P_{22}(\bar y): E^u_{\bar x} \to  E^u_{F(\bar x)}$
  are all linear maps.






Let $(u,v) = (t, \varphi_{\bar x}(t)),\  n=0,1, \cdots$. The invariance
 under   $\FF_{\bar x}$ requires that  $\varphi_{\bar x}(t) $ satisfies
$$\varphi_{F(\bar x)}[P_{11}(\bar x) t + P_{12}(\bar x)\varphi_{\bar x}
(t) + g_{1, \bar x}(t, \varphi_{\bar x}(t))] $$
$$= P_{21}(\bar x)t + P_{22}(\bar x)\varphi_{\bar x}(t) + g_{2, \bar x}
(t, \varphi_{\bar x}(t)).\eqno(4.2)$$ 

We consider the space $\SS$ of all continuous maps from $B^s_{\gamma}
(\bar x)$ to
 $B^u_{\gamma}(F(\bar x))$ with $\bar x$ as a parameter
$$\SS : \{ \phi_{\bar x}(t) | \phi_{\bar x}(t) : B^s_{\gamma}(\bar x)
 \to  B^u_{\gamma}(F (\bar x)); \phi_{\bar x} (t) \ \hbox{\rm is\  
continuous \ in \ }\bar x \ \hbox{\rm and } \ t  \} $$
With the norm $\| \phi_{\bar x}(t) \| = \sup_{\bar x  \in \Delta} 
\sup_{t \in B^s_{\gamma} } \| \phi_{\bar x}(t) \|, $ this space is a 
Banach space. Define
the operator $\TT$ from $\SS$ into itself by
$$(\TT \phi_{\bar x})|_{\bar x}(t) =P^{-1}_{22}(\bar x)(\phi_{F(\bar x)}
 (P_{11}(\bar x) t + P_{12}(\bar x)\phi_{\bar x}(t) + g_{1, \bar x}
(t, \phi_{\bar x} (t))))$$
$$ - P^{-1}_{22}(\bar x)\cdot
P_{21}(\bar x) t -  P^{-1}_{22}(\bar x)\cdot  g_{2, \bar x}(t, \phi_{\bar x}
 (t)).$$
 By the usual argument,
one can see that $\TT$ is a contraction in a neighborhood of $0$ and the
 unique fixed point   $\varphi_{  \bar x}(t)  $ satisfies $(4.2)$. 
In fact, $\varphi_ { \bar x}(t)  =lim_{m \to \infty} \TT^m 0$, where 
$0$ is the 
zero map from  $B^s_{\gamma}(\bar x)$ to
 $B^u_{\gamma}(F(\bar x))$. 

Now, let us fix a point $\bar x$. We wish to show that $\exp_{\bar y} 
\varphi_{\bar y}(t) $  H\"older continuously depends on 
$\bar y$ when $\bar y \in V^u(\bar x)$ is close to $\bar x$.  For any
 $\bar y$ sufficiently close to $\bar x$, we may consider
 all maps $\varphi_{\bar y}(t)$  as maps from $B^s_{\gamma}(\bar x)$ 
to $B^u_{\gamma}(\bar x)$ and rewrite the transformation  $\FF_{\bar y}$ 
into a matrix form using
the exponential splitting at $\bar x$. For any $\bar \xi = (u, v) \in
 B_{\gamma}( \bar x) \subset B^s_{\gamma}(\bar x) \oplus B^u_{\gamma}
(\bar x),$
$$\FF_{\bar y} \cdot \pmatrix{u \cr 
                     v \cr}= D\FF_{\bar y} \cdot \pmatrix{u \cr 
                     v \cr} + \pmatrix{g_{1,\bar y}(u,v) \cr 
 g_{2, \bar y}(u,v) \cr}.$$   
We have that  
$$ D\FF_{\bar y} =\pmatrix{A_{11}(\bar y) & A_{12}(\bar y)\cr
                A_{21}(\bar y) & A_{22}(\bar y)\cr }$$ 

Note that  $D\FF_{\bar y} = D\exp^{-1}_{F(\bar y)} \cdot D\Phi
\cdot D\exp_{\bar y} =  D\exp^{-1}_{F(\bar y)} \cdot DF \cdot DG 
\cdot D\exp_{\bar y}.$ Since the diffeomorphism $G$ is $C^2$ and 
short ranged, by the virtue of Lemma 4, $DG$ is Lipschitz continuous
 in both the Finsler metric
and the metric $\rho_q$ with   Lipschitz constants arbitrarily close 
to one. This implies
that  for any fixed $\bar y$ both $ A_{11}(\bar y)$ and 
$ A^{-1}_{22}(\bar y)$ are contracting maps in the metric $\rho_q$ 
for $\theta < q \leq 1$. The contracting 
constants will be denoted by $k_1 $ and $k_2$ respectively. We  use 
$K_1 $ and $K_2 $ to denote the Lipschitz constants of $A^{-1}_{11}
(\bar y)$ and $A_{22}(\bar y)$
respectively. 

The operator $\TT$ can also be expressed locally as $$\TT 
\phi_{\bar y}|_{\bar y}(t) =A^{-1}_{22}(\bar y)(\phi_{F(\bar y)}
(A_{11}(\bar y) t + A_{12}(\bar y)\phi_{\bar y}(t) + g_{1, \bar y}
(t, \phi_{\bar y}(t))))$$
$$ - A^{-1}_{22}(\bar y)\cdot
A_{21}(\bar y) t -  A^{-1}_{22}(\bar y)\cdot  g_{2, \bar y}
(t, \phi_{\bar x}(t)),$$
and  $\varphi_{ \bar y}(t) =lim_{m \to \infty} \TT^m 0$. We want 
to show that
$$   \sup_{t \in B^s_{\gamma}(\bar x) } \| (\varphi_{\bar y_1}(t)) -
 (\varphi_{\bar y_2}(t))\|_q \leq
C \cdot  {\rho_q}^{\alpha}(\bar y_1, \bar y_2).\eqno(4.3)$$ 

We   prove that $(4.3)$ holds for $\TT^m 0, \ m=0, 1,2, \cdots$ by
induction. Then, by taking the limit of this sequence, we have the 
desired result. For convenience, we  write $\TT^m 0 = \varphi^m_{ \bar y}
(t) $.

For $m=0$, $(t,\varphi^0_{\bar y}(t))$ is the stable subspace of
$T_{\bar y}\MM$.  So, (4.3) is obviously satisfied since the exponential
 splitting for $DF$ is
H\"older continuous in the metric $\rho_q$.
Assume (4.3) is true for $m=n-1$.
Then,$$\varphi^{n}_{\bar y}(t)= 
 A^{-1}_{22}(\bar y)( \varphi^{n-1}_{F(\bar y)}(A_{11}(\bar y) t +
 A_{12}(\bar y)\varphi^{n-1}_{\bar y}(t) + g_{1,\bar y}(t, 
\varphi^{n-1}_{\bar y}(t)))) $$
$$-  A^{-1}_{22}(\bar y)\cdot
A_{21}(\bar y) t -  A^{-1}_{22}(\bar y)\cdot  g_{2,\bar y}(t,
 \varphi^{n-1}_{\bar y}(t)).$$

Let us denote $$\Sigma_j= A_{11}(\bar y_j) t + A_{12}(\bar  y_j)
\varphi^{n-1}_{\bar y_j}(t) + g_{1,\bar y_j}(t, \varphi^{n-1}_{\bar y_j}
(t)),\  j=1,2$$
Thus,
 $$\|\varphi^n_{\bar  y_1}(t) -\varphi^n_{\bar y_2}(t)\|_q 
\leq
\|A_{22}^{-1}(\bar y_1)  \varphi^{n-1}_{F(\bar y_1)}(\Sigma_1) - 
A_{22}^{-1}(\bar y_2) \varphi^{n-1}_{F(\bar y_2)}(\Sigma_2)\|_q
$$
$$
+ \| A_{22}^{-1}(\bar y_1)A_{21}(\bar y_1)t  - A_{22}^{-1}(\bar y_2)
A_{21}(\bar y_2)t\|_q$$
$$
+ \|A^{-1}_{22}(\bar y_1)\cdot  g_{2,\bar y_1}(t, \varphi^{n-1}_{\bar y_1}
(t))
-A^{-1}_{22}(\bar y_2)\cdot  g_{2,\bar y_2}(t, \varphi^{n-1}_{\bar y_2}
(t))\|_q.\eqno(4.4)$$
By assumption there exist constants $C>0$, $0< \alpha < 1$ such that
$$\|\varphi^{n-1}_{\bar y_1}(t) -\varphi^{n-1}_{\bar y_2}(t)\|_q \leq
C \cdot {\rho_q}^{\alpha}(\bar y_1, \bar y_2)$$ for all $t \in B^s_{\gamma}
(\bar x)$.
In the last step   we   estimate those three  terms involved in (4.4). 

{\it Step 3} \qquad  \quad We first consider
 $g_{1,\bar y}(t, \varphi^{n-1}_{\bar y}(t))$ and $g_{2,\bar y}(t, 
\varphi^{n-1}_{\bar y}(t))$. Note that 
$$\pmatrix { g_{1,\bar y}(u,v) \cr
              g_{2,\bar y}(u,v)\cr} =( \FF_{\bar y}  -D\FF_{\bar y})
\pmatrix{u \cr v \cr}.$$
and for each fixed $\bar y$,  $\FF_i -D\FF_{\bar y} $ is a $C^1$, shift
 invariant,
and  short ranged map with a Lipschitz constant
$\eps_1$, which   can be taken arbitrarily small when
$\gamma$, the radius of the ball $B_{\gamma}(\bar x)$, is small. By 
 similar arguments
 used in proving Lemma 4, one can show that $g_{j,\bar y}, j=1,2$ are
also Lipschitz in the metric $\rho_q$  and the Lipschitz constant
in the  metric   $\rho_q$, denoted by $\eps_2$, approaches zero when
 $\eps_1 \to 0$.
Moreover, since $\Phi = F \cdot G$ is $C^2$, by Lemma 2,  we have
$g_{j,\bar y}$
is also  Lipschitz with respect to $\bar y$ in the  metric $\rho_q$. 
We use $L_1 $ to denote a common bound for these two  Lipschitz constants.




  There exists a constant $\eps_3>0$ such that 
$\|A_{12}(\bar y)\|_q \leq \eps_3$ and $\|A_{21}(\bar y)\|_q \leq \eps_3$ 
for any $\bar y$
close to $\bar x$. In fact $\eps_3$ can be taken arbitrary small. Also one
 can easily see
that $A_{ij}(\bar y)$ are all Lipschitz continuous with respect to 
$\bar y$ in  metric $\rho_q$. We will use $K_3$ to denote the common 
bound of all four Lipschitz constants.


Therefore,
$$ \|A^{-1}_{22}(\bar y_1)\cdot  g_{2,\bar y_1}(t,\varphi^{n-1}_{\bar y_1}(t))
-A^{-1}_{22}(\bar y_2)\cdot  g_{2,\bar y_2}(t, \varphi^{n-1}_{\bar y_2}(t))\|_q
$$
$$
\leq \| A^{-1}_{22}(\bar y_1)\cdot  g_{2,\bar y_1}(t,\varphi^{n-1}_{\bar y_1}
(t))
- A^{-1}_{22}(\bar y_1)\cdot  g_{2,\bar y_2}(t,\varphi^{n-1}_{\bar y_1}
(t))\|_q$$
$$+\ 
\| A^{-1}_{22}(\bar y_1) [  g_{2,\bar y_2}(t,\varphi^{n-1}_{\bar y_1}(t)) 
 - g_{2,\bar y_2}(t, \varphi^{n-1}_{\bar y_2}(t))\|_q 
$$
$$+ \ 
 \|[  A^{-1}_{22}(\bar y_1) - A^{-1}_{22}(\bar y_2)]g_{2,\bar y_2}(t, 
\varphi^{n-1}_{\bar y_2}(t))\|_q$$
$$\leq k_2 L_1 \rho_q(\bar y_1, \bar y_2) + k_2 \eps_2 \|
\varphi^{n-1}_{\bar y_1}(t) -\varphi^{n-1}_{\bar y_2}(t)\|_q 
+ L_2 K_3 \rho_q(\bar y_1,\bar  y_2)$$
$$\leq k_2 \eps_2 C \rho_q^{\alpha}(\bar y_1,\bar  y_2) + L'_1 
\rho_q(\bar y_1,\bar  y_2)$$ where $L_2$ denotes the bound of the
$\rho_q$ norms of $g_{j, y}, j=1,2$ \ in the  metric   $\rho_q$ and 
$L'_1 = k_2 L_1 + L_2 K_3$.
For the second term in (4.4) we have
$$ \| A_{22}^{-1}(\bar y_1)A_{21}(\bar y_1)t  - A_{22}^{-1}(\bar y_2)A_{21}
(\bar y_2)t\|_q$$
$$  \| A_{22}^{-1}(\bar y_1)A_{21}(\bar y_1)t  - A_{22}^{-1}(\bar y_1)A_{21}
(\bar y_2)t\|_q
+ \| [A_{22}^{-1}(\bar y_1) - A_{22}^{-1}(\bar y_2)] A_{21}(\bar y_2)t\|_q$$
$$
\leq k_2 K_3\rho_q(\bar y_1, \bar y_2) + K_2 \eps_3 \rho_q(\bar y_1, \bar y_2)
.$$

    \quad Finally, we estimate the first term in (4.4):
$$\|A_{22}^{-1}(\bar y_1)  \varphi^{n-1}_{F(\bar y_1)}(\Sigma_1) - A_{22}^{-1}
(\bar y_2) \varphi^{n-1}_{F(\bar y_2)}(\Sigma_2)\|_q$$
$$\leq  \|A_{22}^{-1}(\bar y_1)  \varphi^{n-1}_{F(\bar y_1)}(\Sigma_1) -
 A_{22}^{-1}(\bar y_1) \varphi^{n-1}_{F(\bar y_2)}(\Sigma_2)\|_q
+ \|[A_{22}^{-1}(\bar y_1)-A_{22}^{-1}(\bar y_2)] \varphi^{n-1}_{F(\bar y_2)}
(\Sigma_2)\|_q$$
$$\leq k_2 \|\varphi^{n-1}_{F(\bar y_1)}(\Sigma_1) -\varphi^{n-1}_{F(\bar y_2)}
(\Sigma_2)\|_q + K_2 L_3 \rho_q(\bar y_1, \bar y_2)$$
$$\leq k_2 \|\varphi^{n-1}_{F(\bar y_1)}(\Sigma_1) -\varphi^{n-1}_{F(\bar y_2)}
(\Sigma_1)\|_q + k_2\|\varphi^{n-1}_{F(\bar y_2)}(\Sigma_1)
-\varphi^{n-1}_{F(\bar y_2)}(\Sigma_2)\|_q +  K_2 L_3 \rho_q(\bar y_1, 
\bar y_2)$$
$$\leq k_2 C \rho_q^{\alpha}(\bar y_1,\bar  y_2)+ k_2 L_4 \| \Sigma_1 - 
\Sigma_2\|_q +  K_2 L_3 \rho_q(\bar y_1, \bar y_2)
.$$
 where $L_3$
is the bound of the norms of $\varphi^{n-1}_{F(\bar y_2)}(t)$ and $L_4$
 is the Lipschitz 
constant of $\varphi^{n-1}_{F(\bar y_2)}(t)$ with respect to $t$ in the 
 metric   $\rho_q$.
Since we already know that $(\varphi^m_{\bar y})$ converges to
 $\varphi_{\bar y}$, these two constants $L_3, $ and $ L_4$ can be chosen
independent of $\bar y $ and $m$.

On the other hand
 $$\| \Sigma_1 - \Sigma_2\|_q =
 \|A_{11}(\bar y_1) t + A_{12}(\bar y_1)\varphi^{n-1}_{\bar y_1)}(t) +
 g_{1,\bar y_1}(t, \varphi^{n-1}{i,\bar y_1}(t))$$
$$
- [ A_{11}(\bar y_2) t + A_{12}(\bar y_2)\varphi^{n-1}_{\bar y_2}(t) +
 g_{1,\bar y_2}(t, \varphi^{n-1}_{\bar y_2}(t))]\|_q$$
$$\leq \|A_{11}(\bar y_1) t -A_{11}(\bar y_2) t\|_q + \| A_{12}(\bar y_1)
\varphi^{n-1}_{i,y_1}(t) -A_{12}(\bar y_2)\varphi^{n-1}_{\bar y_2}(t)\|_q$$
$$+ \|g_{1,\bar y_1}(t, \varphi^{n-1}_{\bar y_1}(t))- g_{1,\bar y_2}
(t, \varphi^{n-1}_{\bar y_2}(t))\|_q$$
$$\leq K_3 \rho_q(\bar y_1, \bar y_2) + [\eps_3 C  \rho_q^{\alpha}
(\bar y_1, \bar y_2) + K_3 L_3
\rho_q(\bar y_1, \bar y_2) ] + \eps_2 C \rho_q^{\alpha}(\bar y_1, \bar y_2).$$
Combining  all these estimations together we have 
$$\|\varphi^n_{\bar y_1}(t) -\varphi^n_{\bar y_2}(t)\|_q 
\leq [ k_2 C + K_4 \rho_q^{(1-\alpha)}(\bar y_1,\bar y_2) + K_5\eps_4] 
\rho_q^{\alpha}(\bar y_1, \bar y_2),$$ 
where $\eps_4$, depending  on $\eps_1, \eps_2, $ and $\eps_3$,  can be
 taken arbitrarily small  and $K_4, K_5$ are two constants. Thus, if
 $\rho(\bar y_1, \bar y_2)$ is chosen to be sufficiently small, 
we have $$ k_2 C + K_4 \rho_q^{(1-\alpha)}(\bar y_1,\bar y_2) + K_5  
\eps_4 \leq C.$$ 
This concludes the proof of
Theorem 4.












\vskip.5cm

{\bf Proof of Theorem 5} \qquad
We first observe that the $\integer^2$ action $\tau$ induced by
 $(F,S)$ is expansive on $(\Delta, \rho_q)$ for any $0 < q <1$ 
and the conjugacy maps
$h$ and $h^{-1}$ are both uniformly continuous in the  metric  
 $\rho_q,\  \  0<q<1$.
Thus, the $\integer^2$-action $\tau$ induced by $(\Phi,S)$ is 
also expansive in
metric $\rho_q$ on $\Delta_{\Phi}$. Then, Theorem 5 becomes a 
direct corollary
of Proposition 1.
  It is easy to see that for any $0< q_1 < q_2 <1$, the metrics
$\rho_{q_1}$ and $\rho_{q_2}$ are  H\"older equivalent, by which 
we mean that the following inequality holds for some constants
 $C>0$ and $0<b<1$:
$$ \rho_{q_2} (\bar x, \bar y) \leq C \rho^b_{q_1} (\bar x,\bar y).
 $$ Therefore,
the equilibrium states  for $\varphi$ are independent of the choices of the
metric $\rho_q, \ 0<q<1$.




 

{\bf Proof of Lemma 6.1} \qquad Properties 1 and 2 are obvious.

 Let us denote the boundary of the Markov Partition 
$\cup_{i=1}^m R_i$ of $\Lambda$ by $\partial R$, then the boundary of 
the Markov partition of $\Delta$ is $\BB = \cup_{i \in \integer} \BB(i)$, 
where  
$$\BB(i)= \{ \bar x =(x_j)_{j \in \integer} : x_i \in \partial R\}.$$
Property 3 follows directly from the fact that $\pi: \Sigma_A\backslash 
\pi^{-1}(\partial R) \to  \Lambda $ is injective.



{\bf Proof of Lemma 6.2} \qquad 1) Let $\UU=(U_i)$ be an open finite covering
of $\Delta$. The the collection of sets  ${\bar \pi}^{-1}(\UU) = 
({\bar \pi}^{-1}(U_i))$ is an open cover of
$\Sigma_A^{\integer}$. Note that 
$$ P_{\tau}(\varphi) = \sup_{\UU} P_{\tau}(\varphi, \UU) =
\sup_{\UU}(\lim_{n,m \to \infty} {1 \over nm} \log Z_{X_{n,m}}(\varphi, \UU))
$$
and that
$$Z_X(\varphi, \UU) = \min_{(B_j)}\{ \sum_j \exp[ \inf_{\bar y \in B_j} 
\sum_{x \in X}
\varphi ( \tau^x \bar y)]\}$$
$$= \min_{({\bar \pi}^{-1}B_j)}\{ \sum_j \exp[ \inf_{\bar \xi \in
 {\bar \pi}^{-1}B_j} 
 \sum_{x \in X} \varphi^*( \tau \bar \xi)\}= Z_X(\varphi^*, 
{\bar \pi}^{-1}(\UU) ).$$
 We have $P_{\tau}(\varphi) \leq P_{\tau^*}(\varphi^*)$.

2) We need only to observe that $\bar \pi: \Sigma_A^{\integer} \to \Delta$
 is 
one-to-one except for those points in $ {\bar \pi}^{-1}(\BB)$ and 
$\mu(\BB)= \mu^*({\bar \pi}^{-1}(\BB)) = 0$.

 {\bf Proof of Theorem 6}
\qquad 1) 
By Lemma 6.2 
 $h_{\tau}(\mu) + \int \varphi d \mu  = h_{\tau}(\mu^*)  +
 \int \varphi d \mu^* = P_{\tau}(\varphi^*) \geq P{\tau}(\varphi) $.
 This means $\mu$ is an equilibrium state for $\varphi$ and
 $ P_{\tau}(\varphi^*) = P{\tau}(\varphi) $.


2) We first use Hahn-Banach theorem to show that for any probability
 measure
$\mu$ $\tau$-invariant on $\Delta$, there exists a $\tau$-invariant
probability
measure $\nu$ on $\Sigma_A^{\integer}$ with $\mu (E) = \mu^*
 ({\bar \pi}^{-1}(E))$ for any Borel set $E \subset \Delta$.

Consider the linear functional  on a subspace of $C(\Sigma_A^{\integer})$
defined by $ g \bar \pi \to \int g   d \mu$, where $g \in C(\Delta, \rho_q)$.
 This functional is positive and its norm is $1$. Thus it corresponds to
 a probability measure $\beta$ on  $\Sigma_A^{\integer}$. The relation
 $\int g \bar \pi d \beta = \int g d\mu$ implies $\beta({\bar \pi}^{-1}(E)) 
= \mu(E)$. However, $\beta$ may be not  $\tau$-invariant on 
$\Sigma_A^{\integer}$.
We define 
$$\nu :=weak^* -\lim_{(n,m)\to \infty} {1 \over nm}(\sum_{x \in X_{n,m}}
\tau^x \beta ).$$ 
Then, $\nu$ is $\tau$-invariant and we still have 
 $\mu (E) = \nu ({\bar \pi}^{-1}(E))$. Thus 
$$\int g \bar \pi d\nu = \int g d\mu.\eqno{(6.1)}$$

 Now by Lemma 6.2 $h_{\tau}(\nu) + \int \varphi^* d \nu \geq 
h_{\tau}(\mu) + \int \varphi d \mu  = P_{\tau}(\varphi) = P_{\tau}(\varphi^*)$.
Thus $\nu$ is an equilibrium state. So, we set $\mu^* = \nu$.


{\bf Proof of Theorem 7}\qquad
 1) We follow the proof of a similar property in the finite dimensional case by
Bowen [B]. Let us consider the boundary points of the Markov Partition 
of $\Lambda$:     $\partial R = \partial^sR \cup  \partial^uR $, where $$ 
\partial^sR = \cup_{i=1}^m\{ x \in R_i:  x \not\in \hbox{\rm interior \ of \ }
 V^u(x) \cap R_i\};$$
$$
 \partial^uR = \cup_{i=1}^m\{ x \in R_i:  x \not\in \hbox{\rm interior \ of \ } 
V^s(x) \cap R_i\}.$$
Then the boundary of the Markov partition of $\Delta$ \  $\BB =
 \cup_{i \in \integer}
 \BB(i)$, where  
$$\BB(i)= \{ \bar x =(x_j)_{j \in \integer} : x_i \in \partial R\}.$$
Let $\BB^s(i)=  \{ \bar x =(x_j)_{j \in \integer} : x_i \in \partial^s R\}$ and
$\BB^u(i)=  \{ \bar x =(x_j)_{j \in \integer} : x_i \in \partial^u R\}$. In 
order to show
$\mu^*({\bar \pi}^{-1}(\BB))=0$, we will show that for each $i$,  
$\mu^*({\bar \pi}^{-1}(\BB^s(i)))=0$ and   $\mu^*({\bar \pi}^{-1}(\BB^u(i)))=0$. 

  Consider $D_s(i)= {\bar \pi}^{-1}(\BB^s(i))$. $D_s(i)$ is a closed subset
of $\Sigma_A^{\integer}$ and $\sigma^t D_s(i) \subset D_s(i).$ As $\mu^*$ is 
$\sigma^t$ invariant, $\mu^*(\sigma_t)^n  D_s(i) = \mu^*( D_s(i))$ for any
 $ n \in \natural$. Since $(\sigma^t)^{n +1} D_s(i) \subset (\sigma^t)^n 
 D_s(i)$, one has $$\mu^*(\cap_{n \geq 0} (\sigma^t)^n  D_s(i) ) = 
\mu^*( D_s(i)).$$
Now $\mu^*$ is $\sigma^t$ ergodic and positive on open set and the the 
set  $\cap_{n \geq 0} (\sigma^t)^n  D_s(i) $ is 
 $\sigma^t-$invariant and closed . Then, $\cap_{n \geq 0} (\sigma^t)^n  
D_s(i) $ has measure zero\  $\mu^*(D_s(i)) =0$.
    Similarly one can show that   $\mu^*({\bar \pi}^{-1}(\BB^u(i)))=0$.

 2)   Let $\mu^*$ be a Gibbs state for a H\"older continuous function 
$\psi$ on $\Sigma_A^{\integer}$.
  Without loss of generality,  we will prove $\mu^*({\bar \pi}^{-1}
(\BB^s(0)))=0$.

Note that $\partial^sR$ is a finite union of local stable manifolds 
intersecting with $\Lambda$. Let us define the following subsets of
 $\Sigma_A^{\integer}$.
For each fixed element $\xi^* \in \Sigma_A$ and $k \in \integer$
 $$ E_k(\xi^*)= \{ \bar \xi = (\xi_i): \xi_i \in \Sigma, i \in \integer,
 \xi_0(j) = \xi^*(j), j \leq k \}.$$
One can see that the set ${\bar \pi}^{-1}(\BB^s(0))$ is a subset of a  
finite union of the sets  defined above. So  it suffices   to show that
 $\mu^*(E_k(\xi^*) ) =0$. Without loss of generality we will further 
assume $k=0$ and $\xi^*$ is   fixed. We consider the following sequence
 of sets that converges to $E_0 (\xi^*)$.
$$ E^{m} = \{ \bar \xi = (\xi_i): \xi_i \in \Sigma, i \in \integer,
 \xi_0(j) = \xi^*(j),  -m \leq j \leq 0 \}.$$
One can easily see that $ \lim_{m \to \infty} \mu^*(E^{(m)}) = 
\mu^*(E_0(\xi^*) )$. Next
we estimate \hb $\mu^*( E^{(m)})$.

Since the set of all Gibbs states for $\psi$ is the closed convex hull 
of the thermodynamic limits of the Gibbs distributions, we may assume 
that $\mu^*$ is   such a limit, i.e., $\lim_{n \to \infty} \mu^*_n =
 \mu^*$, where   $\mu^*_n$ are the measures on $\Sigma_A^\integer$ 
determined by the Gibbs distributions
 $$ p_{\scriptscriptstyle X_n}(\bar \xi_{\sst X_n}, \bar \eta^*_{\sst X^C_n}) 
= {  1
\over
\sum_{\bar \eta: \bar \eta|_{X_n^C} = \bar \eta^* |_{ X_n^C}} 
\exp(    \sum _{x \in \integer^2 } \psi(\tau^x \bar \eta) -
 \psi(\tau^x (\bar \xi_{\sst X_n}, \bar \eta^*_{\sst X^C_n}))) }$$

$$= { \exp (\sum_{x \in \integer^2 }\psi(\tau^x (\bar \xi_{\sst X_n},
 \bar \eta^*_{\sst X^C_n})))
       \over 
\sum_{\bar \eta: \bar \eta|_{\sst X_n^C} = \bar \eta^* |_{\sst X_n^C}} 
\exp(    \sum _{x \in \integer^2 } \psi(\tau^x \bar \eta))} $$
and  $X_n \to \integer^2.$ 
In the above expressions, $\bar \eta^*$ is any fixed configuration 
in $\Sigma_A^\integer$, $\bar \xi_{\sst X_n}$ is the restriction of 
the  configuration $\bar \xi$ to the subset
 $X_n$ and $\bar \eta^*_{\sst X^C_n}$
 is the restriction of $\bar \eta^*$  to $X^C_n$.

For convenience we introduce the following notation.   
Let $N$ be the smallest positive integer such that every entry of the matrix
$A^N$ is positive. $V_0= \{ (0,j) \in \integer^2,  j \in \integer\}$.  
$S_{m+N} = \{ (0,j) \in \integer^2,  -m-N \leq j \leq N\} $. $W_n = X_n 
\cap V_0$.  We  assume $ X_n \supset S_{m+N} $.  Thus
$$ \mu_n^*(E^{(m)}) = { \sum_{ \bar \eta:\  \bar \eta|_{X_n^C}= \bar
 \eta*|_{X_n^C},\ 
\bar \eta|_{S_m}= \xi^*|_{S_{m}}} \exp (\sum_{x \in \integer^2}
 \psi(\tau^x \bar \eta))            \over
\sum_{ \bar \eta: \ \bar \eta|_{X_n^C}= \bar \eta*|_{X_n^C}
 } \exp( \sum_{x \in \integer^2} \psi(\tau^x \bar \eta))    } $$
$$= {
\sum_{ \bar \eta_{ \sst { X_n \backslash V_0}} \  } 
    \sum_{\bar \eta_{\scriptscriptstyle W_n \backslash S_{m}}: 
\bar \eta|_{ \scriptscriptstyle S_{m}} =\xi^*|_{\scriptscriptstyle 
S_{m}}  } 
\exp( \sum_{x \in \integer^2} \psi(\tau^x \bar \eta)) 
                          \over 
  \sum_{ \bar \eta_{\scriptscriptstyle X_n \backslash V_0 } \ }    
   \sum_{\bar \eta_{\scriptscriptstyle  W_n   }\ }
      \exp( \sum_{x \in \integer^2} \psi(\tau^x \bar \eta))   },
$$
where  the sum $\sum_{ \bar \eta_{X_n \backslash V_0}  }$  is   taken 
over all configurations $\bar \eta $ on $X_n \backslash V_0$ with 
$\bar \eta|_{X_n^C}=\bar \eta^*_{X_n^C}$. The restriction of any
 configuration in the above expressions to   $X^C_n$ is always 
$\bar \eta^*_{X_n^C}$. Other sums are defined in a similar way.

 Now we estimate the following quotient

$$ {   \sum_{\bar \eta_{\scriptscriptstyle W_n \backslash S_{m}}: 
\bar \eta|_{ \scriptscriptstyle S_{m}} =\xi^*|_{\scriptscriptstyle S_{m}} }
      \exp( \sum_{x \in \integer^2} \psi(\tau^x \bar \eta))
\over
     \sum_{\bar \eta_{\scriptscriptstyle  W_n   }\ } 
      \exp( \sum_{x \in \integer^2} \psi(\tau^x \bar \eta))
}$$
$$= { \sum_{ \bar \eta_{  \sst{W_n} \backslash \sst{S_{m+N}}  }  }
\sum_{\bar \eta_{\sst{S_{m+N}}}:  \bar \eta|_{ \sst{ S_{m}} } =
\xi^*|_{\sst{ S_{m}}  }  }
\exp( \sum_{x \in \integer^2} \psi(\tau^x \bar \eta))
\over
\sum_{ \bar \eta_{\sst{ W_n \backslash S_{m+N} } }     } 
\sum_{\bar \eta_{\sst{S_{m+N}}  } }
 \exp( \sum_{x \in \integer^2} \psi(\tau^x \bar \eta))  }. $$
Let $$Q_1= { \sum_{\bar \eta_{\sst{S_{m+N}}}:  \bar \eta|_{ \sst{ S_{m}} }
 =\xi^*|_{\sst{ S_{m}}  }  }
\exp( \sum_{x \in \integer^2} \psi(\tau^x \bar \eta))
\over
\sum_{\bar \eta_{\sst{S_{m+N}}  }  }
 \exp( \sum_{x \in \integer^2} \psi(\tau^x \bar \eta))  }. $$
Let $P$ denote the size of the matrix $A$. 
Then,
 $$   Q_1 \leq
P^{N} \max_{\bar \eta_{\sst{X_n} \backslash \sst{S_m} }  } 
{  \exp(  \sum_{x \in \integer^2} \psi ( \tau^x ( \xi^*_{\sst S_m},
\bar \eta|_{\sst X^C_n \backslash \sst {S_m} }) )
\over 
\sum_{\bar \eta_{\sst{S_m}} } 
 \exp(  \sum_{x \in \integer^2} \psi ( \tau^x (\bar \eta_{\sst S_m}, 
\bar \eta|_{\sst X^C_n \backslash \sst {S_m}  }  ) )   }
,
$$
where the maximum is taken over all $\bar \eta $ on ${{X_n} \backslash {S_m} }$.

We see that $$ Q_2 = {  \exp(  \sum_{x \in \integer^2} \psi 
( \tau^x ( \xi^*|_{\sst S_m}, \bar \eta|_{\sst X^C_n \backslash \sst {S_m} }) )
\over 
\sum_{\bar \eta_{\sst{S_m}} } 
 \exp(  \sum_{x \in \integer^2} \psi ( \tau^x (\bar \eta|_{\sst S_m}, 
\bar \eta|_{\sst X^C_n \backslash \sst {S_m} }) )}$$ 
$$= {1 \over 
\sum_{\bar \eta_{\sst{S_m}} } 
 \exp(  \sum_{x \in \integer^2} \psi ( \tau^x (\bar \eta|_{\sst S_m},
 \bar \eta|_{\sst X^C_n \backslash \sst {S_m} }) - \psi ( \tau^x 
( \xi^*|_{\sst S_m}, \bar \eta|_{\sst X^C_n \backslash \sst {S_m} }) )  } .$$
One can see that there exists an $\eps_1$ independent of $m$ and $X_n$ 
such that 
$$   \sum_{x \in \integer^2 \backslash S_m} |\psi ( \tau^x 
(\bar \eta|_{\sst S_m}, \bar \eta|_{\sst X^C_n \backslash \sst {S_m} }) 
- \psi ( \tau^x ( \xi^*|_{\sst S_m}, \bar \eta|_{\sst X^C_n \backslash
 \sst {S_m} })| \leq \eps_1 m $$ and $\eps_1 $ can be taken   small if $c$
 is small. Thus 
$ Q_2 \leq  Q_3 \exp{\eps_1m}$, where
$$Q_3= {  \exp(  \sum_{x \in S_m} \psi ( \tau^x ( \xi^*|_{\sst S_m}, 
\bar \eta|_{\sst X^C_n \backslash \sst {S_m} }) )
\over 
\sum_{\bar \eta_{\sst{S_m}} } 
 \exp(  \sum_{x \in S_m} \psi ( \tau^x (\bar \eta|_{\sst S_m}, 
\bar \eta|_{\sst X^C_n \backslash \sst {S_m} }) )}$$ 
is   a Gibbs distribution
 on $\Sigma_A$.  Let us arbitrarily fix a configuration $\bar \eta_1$ 
over $\integer^2 \backslash V_0 $. Let $\nu$ be the unique Gibbs state 
for
$\psi_{\bar \eta_1 }= \psi({\bar \eta_{\sst{V_0}}, \bar \eta_1 }) $. 
Then, when $m$ is sufficiently large, there exists $\eps_2 >0 $
such that 
$ {1 \over m} \log Q_3 $
$$= {1 \over m }  \sum_{x \in S_m} \psi ( \tau^x ( \xi^*|_{\sst S_m},
 \bar \eta|_{\sst X^C_n \backslash \sst {S_m} }) -
 {1 \over m } \log \sum_{\bar \eta_{\sst{S_m}} } 
 \exp(  \sum_{x \in S_m} \psi ( \tau^x (\bar \eta|_{\sst S_m}, 
\bar \eta|_{\sst X^C_n \backslash \sst {S_m} }) ) 
$$
$$ \leq \int \psi_{\bar \eta_1 } d\nu - P(  \psi_{\bar \eta_1 } ) + \eps_2
= - h_{\nu}+ \eps_2 ,$$
where $ P(  \psi_{\bar \eta_1 } )$ is the topological presure over
 $\Sigma_A$
, $h_{\nu} >0 $ is the metric entropy, and $\eps_2 \to 0$
when $c \to 0, m \to \infty$.

Thus, $Q_3 \leq \exp{  (- h_\nu + \eps_2) m   }$ and 
$ Q_1 \leq P^{N} \exp{  (- h_\nu + \eps_1 + \eps_2) m   }$. Therefore,
 $ \mu^*( E_0{(\xi^*)})=\lim_{m \to \infty} \mu^*( E^{m})  =0$.






 

The statements 1 and 2 of Theorem 8  are  direct consequences of
Proposition 3 and Theorems 6 and 7.  The mixing property with
 respect to both
$F$ and $S$ comes from the equality $(6.1)$




{\bf ACKNOWLEDGEMENT} \quad   The author  thanks his advisor,  
Professor Yakov B. Pesin, for his guidance, encouragement. 
The author also thanks Professor Pavel M. Bleher  and especially, 
Professor Jean Bricmont for helpful discussions. 





\vfill\eject


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{\it  e-mail:  jiang@math.psu.edu}















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