\documentclass[reqno]{amsart}
\usepackage{hyperref}
\usepackage{epic}

\AtBeginDocument{{\noindent\small
\emph{Electronic Journal of Differential Equations},
Vol. 2011 (2011), No. 100, pp. 1--54.\newline
ISSN: 1072-6691. URL: http://ejde.math.txstate.edu or http://ejde.math.unt.edu
\newline ftp ejde.math.txstate.edu}
\thanks{\copyright 2011 Texas State University - San Marcos.}
\vspace{9mm}}

\begin{document}
\title[\hfilneg EJDE-2011/100\hfil Stability and approximations of
eigenvalues]
{Stability and approximations of eigenvalues and eigenfunctions of
the Neumann Laplacian, part 3}

\author[M. M. H. Pang\hfil EJDE-2011/100\hfilneg]
{Michael M. H. Pang}

\address{Michael M. H. Pang \newline
 Department of Mathematics\\
 University of Missouri-Columbia\\
 Columbia, MO 65211, USA}
\email{pangm@missouri.edu}

\thanks{Submitted November 5, 2010. Published August 7, 2011.}
\subjclass[2000]{35P05, 35P15}
\keywords{Stability; approximations; Neumann eigenvalues 
and eigenfunctions}

\begin{abstract}
 This article is a sequel to two earlier articles (one of them 
 written jointly with R. Banuelos) on stability results for the Neumann 
 eigenvalues and eigenfunctions of domains in $\mathbb{R}^2$ with 
 a snowflake type  fractal boundary. 
 In particular we want our results to be applicable to the Koch snowflake 
 domain. In the two earlier papers we assumed that a domain 
 $\Omega\subseteq\mathbb{R}^2$ which has a snowflake type boundary 
 is approximated by a family of subdomains and that the Neumann heat 
 kernel of $\Omega$ and those of its approximating subdomains satisfy a 
 uniform bound for all sufficiently small $t>0$. The purpose of this 
 paper is to extend the results in the two earlier papers to the 
 situations where the approximating domains are not necessarily 
 subdomains of $\Omega$. We then apply our results to the Koch snowflake 
 domain when it is  approximated from outside by a decreasing sequence of 
 polygons.
\end{abstract}

\maketitle
\numberwithin{equation}{section}
\newtheorem{theorem}{Theorem}[section]
\newtheorem{lemma}[theorem]{Lemma}
\newtheorem{remark}[theorem]{Remark}
\newtheorem{definition}[theorem]{Definition}
\newtheorem{proposition}[theorem]{Proposition}
\allowdisplaybreaks


\section{Introduction} \label{sec:1}

This paper is a sequel to the papers \cite{BP,P2}. The goal of these
three papers is to prove stability results for the Neumann eigenvalues
and eigenfunctions of domains in $\mathbb{R}^2$ with a snowflake
type fractal boundary. In particular we want our results to be applicable
to the Koch snowflake domain. In \cite{BP} and \cite{P2} we assumed
that a domain  $\Omega\subseteq\mathbb{R}^2$ which has a snowflake
type boundary is approximated by a family of subdomains and that the
Neumann heat kernel of $\Omega$ and those of its approximating subdomains
satisfy a uniform bound for all sufficiently small $t>0$ (see Hypothesis
1.1 of \cite{BP} and \cite{P2}). The referee of \cite{BP}
asked whether stability results similar to those in \cite{BP} and
\cite{P2} are still true if the approximating domains of $\Omega$
are not necessarily subdomains of $\Omega$ and whether the proofs
in \cite{BP} and \cite{P2} can be extended to those situations. If the results and methods in \cite{BP} and \cite {P2} can be extended to those situations, then they can be applied to domains, such as the Koch snowflake domain,  which can be approximated by a familiar decreasing sequence of polygons from outside.  The method in \cite{BP,P2} can be
extended to situations when the approximating domains are not necessarily
subdomains of $\Omega$, but not in a straight forward manner. The
purpose of this paper is to work out such an extension and to apply
it to the Koch snowflake domain when it is approximated from  outside
by a decreasing sequence of polygons.

To state our results we first fix notation. Let
$\Omega\subseteq\mathbb{R}^N$, $N\geq2$, be a bounded Sobolev
extension domain. Let $\epsilon_0>0$ be sufficiently small,
depending on $\Omega$. For each $\epsilon\in(0,\epsilon_0]$, let
$\Omega_{\epsilon}$, $\Omega^{\epsilon}$ and $\Omega(\epsilon)$ be
bounded Sobolev extension domains in $\mathbb{R}^N$ satisfying the
following assumptions:
\begin{equation} \label{eq:1.1}
\begin{gathered}
\Omega_{\epsilon}  \supseteq\{ x\in\Omega :\operatorname{dist} (x,\partial\Omega)>\epsilon\},\\
\Omega^{\epsilon}  \subseteq\{x\in\mathbb{R}^N:\operatorname{dist} (x,\Omega)<\epsilon\},\\
\Omega_{\epsilon}
\subseteq\Omega(\epsilon)\subseteq\Omega^{\epsilon}.
\end{gathered}
\end{equation}
We shall assume that
\begin{equation}
\Omega_{\epsilon_1}\supseteq\Omega_{\epsilon_2}\quad \text{if
}0<\epsilon_1\leq\epsilon_2\leq\epsilon_0\label{eq:1.2}\end{equation}
 and that
\begin{equation}
\Omega^{\epsilon_1}\subseteq\Omega^{\epsilon_2}\quad\text{if
}0<\epsilon_1\leq\epsilon_2\leq\epsilon_0.\label{eq:1.3}
\end{equation}
 Let $-\Delta_{\epsilon}$, $-\Delta$, $-\Delta^{\epsilon}$,
$-\Delta(\epsilon)$
be the Neumann Laplacian defined on $\Omega_{\epsilon}$, $\Omega$,
$\Omega^{\epsilon}$ and $\Omega(\epsilon)$, respectively,  and let
$P_{\epsilon}(t,x,y)$, $P(t,x,y)$, $P^{\epsilon}(t,x,y)$ and
$P(\epsilon)(t,x,y)$ be the heat kernel of
$e^{-\Delta_{\epsilon}t}$, $e^{-\Delta t}$,
$e^{-\Delta^{\epsilon}t}$ and $e^{-\Delta(\epsilon)t}$,
respectively. We shall assume that there exists a positive
continuous function $c:(0,1]\to(0,\infty)$ such that for all
$0<\epsilon\leq\epsilon_0$ and all $0<t\leq1$ we have
\begin{equation} \label{eq:1.4}
\begin{gathered}
P_{\epsilon}(t,x,y)  \leq c(t)\quad (x,y\in\Omega_{\epsilon}),\\
P(t,x,y)  \leq c(t)\quad (x,y\in\Omega),\\
P^{\epsilon}(t,x,y)  \leq c(t)\quad (x,y\in\Omega^{\epsilon}),\\
P(\epsilon)(t,x,y)  \leq c(t)\quad (x,y\in\Omega(\epsilon)).
\end{gathered}
\end{equation}
 Since the domains $\Omega_{\epsilon}$, $\Omega$, $\Omega^{\epsilon}$
and $\Omega(\epsilon)$ are assumed to be bounded, \eqref{eq:1.4}
implies that $-\Delta_{\epsilon}$, $-\Delta$, $-\Delta^{\epsilon}$
and $-\Delta(\epsilon)$ all have compact resolvents (see
\cite[Theorem~2.1.5]{D2}). We shall write
$\{\mu_{i}\}_{i=1}^{\infty}$ for the eigenvalues of $-\Delta$,
where $\{\mu_{i}\}_{i=1}^{\infty}$ is a non-decreasing sequence
with $\mu_1=0$ and the eigenvalues are listed repeatedly
according to multiplicity. Similarly, for
$0<\epsilon\leq\epsilon_0$, we shall write
$\{\mu_{i,\epsilon}\}_{i=1}^{\infty}$,
$\{\mu_{i}^{\epsilon}\}_{i=1}^{\infty}$, and
$\{\mu_{i}(\epsilon)\}_{i=1}^{\infty}$ for the eigenvalues of
$-\Delta_{\epsilon}$, $-\Delta^{\epsilon}$ and
$-\Delta(\epsilon)$, respectively. We shall write
$\{\varphi_{i}\}_{i=1}^{\infty}$,
$\{\varphi_{i,\epsilon}\}_{i=1}^{\infty}$,
$\{\varphi_{i}^{\epsilon}\}_{i=1}^{\infty}$ and
$\{\varphi_{i}(\epsilon)\}_{i=1}^{\infty}$ for the corresponding
eigenfunctions of $-\Delta$, $-\Delta_{\epsilon}$,
$-\Delta^{\epsilon}$ and $-\Delta(\epsilon)$, respectively. We
may, and shall, assume that $\{\varphi_{i}\}_{i=1}^{\infty}$,
$\{\varphi_{i,\epsilon}\}_{i=1}^{\infty}$,
$\{\varphi_{i}^{\epsilon}\}_{i=1}^{\infty}$ and
$\{\varphi_{i}(\epsilon)\}_{i=1}^{\infty}$ are complete
orthonormal systems in $L^2(\Omega)$,
$L^2(\Omega_{\epsilon})$, $L^2(\Omega^{\epsilon})$ and
$L^2(\Omega(\epsilon))$, respectively. We define the sequence
$\{k_{i}\}_{i=1}^{\infty}$ of positive integers using the
multiplicities of the eigenvalues $\{\mu_{i}\}_{i=1}^{\infty}$ of
$-\Delta$ as follows:

 Let $k_1=1$ and, for $i=2, 3, 4, \dots$, we define
$k_i$ by:
\begin{equation} \label{eq:1.5}
\begin{split}
0 & =\mu_1<\mu_2=\mu_3=\dots=\mu_{k_2}<\mu_{k_2+1}=\mu_{k_2+2}
=\dots=\mu_{k_3}\\
 & \quad<\mu_{k_3+1}=\mu_{k_3+2}=\dots=\mu_{k_4}<\mu_{k_4+1}
=\dots.\end{split}
\end{equation}
 For all $j=1,2,3,\dots$ and all $\epsilon\in(0,\epsilon_0]$ we
write \begin{equation}
\varphi_{j}|_{\Omega\cap\Omega(\epsilon)}
=\sum_{\ell=1}^{\infty}a_{j,\ell}(\epsilon)\varphi_{\ell}(\epsilon)
\in L^2(\Omega\cap\Omega(\epsilon))
\subseteq L^2(\Omega(\epsilon)).\label{eq:1.6}
\end{equation}
 Let $p\geq1$ be an integer. For $i=k_{p}+1$, $\dots$ , $k_{p+1}$
and $\epsilon\in(0,\epsilon_0]$ let
\begin{equation}
\hat{\psi}_{i}(\epsilon)
=\Big(\sum_{\ell=k_{p}+1}^{k_{p+1}}a_{i,\ell}
(\epsilon)\varphi_{\ell}(\epsilon)\Big)
\Big|_{\Omega\cap\Omega(\epsilon)}\label{eq:1.7}
\end{equation}
and let
\begin{equation}
\psi_{i}(\epsilon)=\|\hat{\psi_{i}}(\epsilon)\|_{L^2
(\Omega\cap\Omega(\epsilon))}^{-1}\hat{\psi}_{i}(\epsilon).
\label{eq:1.8}
\end{equation}
We now state our results:

\begin{theorem}\label{thm:1.1}
For all $i=1,2,3,\dots$, we have
\begin{equation}
\lim_{\epsilon\downarrow0}\mu_{i}(\epsilon)=\mu_{i}.\label{eq:1.9}
\end{equation}
 \end{theorem}

\begin{theorem}\label{thm:1.2}
Let $K$ be a compact subset of $\Omega$. Then we have
\begin{equation}
\lim_{\epsilon\downarrow0}\{\sup_{x\in K}|\varphi_{j}(x)-\psi_{j}
(\epsilon)(x)|\}=0\label{eq:1.10}
\end{equation}
 for $j=1,2,3,\dots$.
\end{theorem}

 To apply Theorems \ref{thm:1.1} and \ref{thm:1.2} to the
Koch snowflake domain, we have

\begin{theorem}\label{thm:1.3}
Let $\Omega\subseteq\mathbb{R}^2$
be the Koch snowflake domain. Let
$\{\Omega_{\rm out}(n)\}_{n=1}^{\infty}$ be the usual decreasing
sequence of polygons approximating $\Omega$ from outside, with
$\Omega_{\rm out}(1)$ being a regular hexagon. Let
$\{\Omega_{\rm in}(n)\}_{n=1}^{\infty}$ be the usual increasing sequence
of polygons approximating $\Omega$ from inside, with
$\Omega_{\rm in}(1)$ being an equilateral triangle. Let
$P^{\Omega}(t,x,y)$, $P^{\Omega_{\rm out}(n)}(t,x,y)$ and
$P^{\Omega_{\rm in}(n)}(t,x,y)$ be the Neumann heat kernels on $\Omega$,
$\Omega_{\rm out}(n)$ and $\Omega_{\rm in}(n)$, respectively. Then there
exists $c\geq1$, independent of $n$, such that
\begin{equation} \label{eq:1.11}
\begin{gathered}
P^{\Omega}(t,x,y)  \leq ct^{-1}\quad (x,y\in\Omega),\\
P^{\Omega_{\rm out}(n)}(t,x,y)  \leq ct^{-1}\quad (x,y\in\Omega_{\rm out}(n)),\\
P^{\Omega_{\rm in}(n)}(t,x,y)  \leq ct^{-1}\quad (x,y\in\Omega_{\rm in}(n)),
\end{gathered}
\end{equation}
for all $0<t\leq1$ and $n=1,2,3,\dots$.
\end{theorem}

\begin{remark} \rm
(i) The third inequality in \eqref{eq:1.11}
was proved in \cite[Theorem 1.3]{P2}.

 (ii) Since $\Omega$, $\Omega_{\rm out}(n)$, $\Omega_{\rm in}(n)$, $n=1,2,3,\dots$,
are bounded Sobolev extension domains, Theorem~\ref{thm:1.3} enables
one to apply Theorems~\ref{thm:1.1} and \ref{thm:1.2} to the case
when $\Omega$ is the Koch snowflake domain approximated from outside
by the sequence $\{\Omega_{\rm out}(n)\}_{n=1}^{\infty}$ by putting
$\{\Omega_{\epsilon}\}=\{\Omega_{\rm in}(n)\}_{n=1}^{\infty}$ and $\{\Omega^{\epsilon}\}=\{\Omega(\epsilon)\}=\{\Omega_{\rm out}(n)\}_{n=1}^{\infty}$.
\end{remark}

 In Section \ref{sec:2} we shall prove some abstract
approximation results for families of non-negative self-adjoint
operators with domains in Hilbert spaces. In Section~\ref{sec:3}
we consider the case when these non-negative self-adjoint
operators are the Neumann Laplacians defined on domains of
$\mathbb{R}^N$. It will be seen that results in
Sections~\ref{sec:2} and \ref{sec:3} imply Theorems~\ref{thm:1.1}
and \ref{thm:1.2}. Theorem~\ref{thm:1.3} will be proved in
Section~\ref{sec:4}.

We refer to the references in \cite{BP,P2} for recent papers on
numerical studies on the Neumann eigenvalues and eigenfunctions of the Koch
snowflake domain and on stability results for Neumann eigenvalues
and eigenfunctions. In addition, we mention the excellent recent survey
paper \cite{BLLC}, and references therein, for stability results
for eigenvalues and eigenfunctions of elliptic operators defined on
domains with either Dirichlet or Neumann boundary conditions.


\section{Quadratic forms and approximations}
\label{sec:2}

In this section we prove the abstract theorems we shall need in the
proofs of the mains results stated in Section~\ref{sec:1}. If $\mathcal{U}$
and $\mathcal{V}$ are Hilbert spaces and if $\mathcal{U}\subseteq \mathcal{V}$, then we shall
denote the orthogonal projection of $\mathcal{V}$ onto $\mathcal{}U$ by $P_{\mathcal{V}, \mathcal{U}}$ and write
$\mathcal{U}^{\bot}\mathcal{V}$ for the orthogonal compliment of $\mathcal{U}$ in $\mathcal{V}$. We shall
also write $I_{\mathcal{U}}$ for the identity map on $\mathcal{U}$. We shall let $\mathcal{H}$
be a fixed Hilbert space. For all sufficiently small $\epsilon>0$,
let $\mathcal{H}_{\epsilon}$ and $\mathcal{H}^{\epsilon}$ be Hilbert
spaces satisfying the following assumptions:
\begin{itemize}
\item [(A1)] If $0<\epsilon_2\leq\epsilon_1$, then
 $\mathcal{H}^{\epsilon_2}\subseteq\mathcal{H}^{\epsilon_1}$.

\item [(A2)] If $0<\epsilon_2\leq\epsilon_1$, then
 $\mathcal{H}_{\epsilon_2}\supseteq\mathcal{H}_{\epsilon_1}$.

\item [(A3)] $\cap_{\epsilon>0}\mathcal{H}^{\epsilon}=\mathcal{H}
 =\cup_{\epsilon>0}\mathcal{H}_{\epsilon}$.

\item [(A4)] For all $f\in\mathcal{H}$ we have
\[
\|f-P_{\mathcal{H}, \mathcal{H}_{\epsilon}}f\|_{\mathcal{H}}\to0
\quad \text{as }\epsilon\downarrow0,
\]
 where $\|\cdot\|_{\mathcal{H}}$ denotes the norm in $\mathcal{H}$.

\item [(A5)] If $\epsilon_1>0$ and if
$f\in\mathcal{H}^{\epsilon_1}$,
then \[
\|P_{\mathcal{H}^{\epsilon_1}, \mathcal{H}}
f-P_{\mathcal{H}^{\epsilon_1}, \mathcal{H}^{\epsilon}}f
\|_{\mathcal{H}^{\epsilon}}\to0 \quad \text{as }\epsilon\downarrow0.
\]

\end{itemize}
For all sufficiently small $\epsilon>0$ let $\mathcal{A}(\epsilon)$
and $\mathcal{B}(\epsilon)$ be Hilbert spaces satisfying the following
assumptions:
\begin{itemize}
\item [(A6)] $\mathcal{H}_{\epsilon}\subseteq\mathcal{B}
(\epsilon)\subseteq\mathcal{H}\cap\mathcal{A}(\epsilon)
\subseteq\mathcal{A}(\epsilon)\subseteq\mathcal{H}^{\epsilon}$,
\item [(A7)] For all $f\in\mathcal{H}$ we have
\[
\|f-P_{\mathcal{H}, \mathcal{B}(\epsilon)}f\|_{\mathcal{H}}\to0
\quad \text{as }\epsilon\downarrow0.
\]

\end{itemize}
We assume that for all sufficiently small $\epsilon>0$ there exists
a closed subspace $\mathcal{C}(\epsilon)$ of $\mathcal{A}(\epsilon)$
satisfying the following assumptions:
\begin{itemize}
\item [(A8)] $\mathcal{C}(\epsilon)\subseteq\mathcal{H}^{\bot}
\mathcal{H}^{\epsilon}$.
\end{itemize}

\begin{lemma}\label{lem:2.1}
If $\epsilon_1>0$, then for all
$f\in\mathcal{H}^{\epsilon_1}$, we have
\[
\|P_{\mathcal{H}^{\epsilon_1},\mathcal{C}(\epsilon)}f
\|_{\mathcal{H}^{\epsilon_1}}\to0 \quad
\text{as }\epsilon\downarrow0.
\]
 \end{lemma}

\begin{proof}
Let $f\in\mathcal{H}^{\epsilon_1}$. Then
\[
\begin{split}
&\|P_{\mathcal{H}^{\bot}\mathcal{H}^{\epsilon},
\mathcal{C}(\epsilon)}(P_{\mathcal{H}^{\epsilon},
\mathcal{H}^{\bot}\mathcal{H}^{\epsilon}}(P_{\mathcal{H}^{\epsilon_1},
 \mathcal{H}^{\epsilon}}f))\|_{\mathcal{H}^{\epsilon_1}}\\
&=    \|P_{\mathcal{H}^{\bot}\mathcal{H}^{\epsilon}, \mathcal{C}(\epsilon)}[(I_{\mathcal{H}^{\epsilon}}-P_{\mathcal{H}^{\epsilon}, \mathcal{H}})(P_{\mathcal{H}^{\epsilon_1}, \mathcal{H}^{\epsilon}}f)]\|_{\mathcal{H}^{\epsilon_1}}\\
&\leq   \|P_{\mathcal{H}^{\bot}\mathcal{H}^{\epsilon}, \mathcal{C}(\epsilon)}\|\|P_{\mathcal{H}^{\epsilon_1}, \mathcal{H}^{\epsilon}}f-P_{\mathcal{H}^{\epsilon _1}, \mathcal{H}}\, f \|_{\mathcal{H}^{\epsilon_1}}\\
&\leq   \|P_{\mathcal{H}^{\epsilon_1},
 \mathcal{H}^{\epsilon}}f-P_{\mathcal{H}^{\epsilon_1},
\mathcal{H}}\, f\|_{\mathcal{H}^{\epsilon_1}}
 \to   0\quad \text{as }\epsilon\downarrow0.
\end{split}
\]
 \end{proof}

 We assume that for all sufficiently small $\epsilon>0$ there exists
a closed subspace $\mathcal{D}(\epsilon)$ of $\mathcal{A}(\epsilon)$
satisfying the following assumptions:
\begin{itemize}
\item [(A9)] $\mathcal{A}(\epsilon)=\mathcal{B}(\epsilon)\oplus\mathcal{C}(\epsilon)\oplus\mathcal{D}(\epsilon)$,
where $\oplus$ denotes orthogonal direct sum.
\item [(A10)] If $\epsilon_1>0$, then, for all $f\in\mathcal{H}^{\epsilon_1}$,
\[
\|P_{\mathcal{H}^{\epsilon_1}, \mathcal{D}(\epsilon)}f\|_{\mathcal{H}^{\epsilon_1}}\to0 \quad \text{as }\epsilon\downarrow0.\]

\end{itemize}
For all sufficiently small $\epsilon>0$ let $Q^{\epsilon}$ and $Q_{\epsilon}$
be non-negative closed quadratic forms with domains $\operatorname{Dom}(Q^{\epsilon})\subseteq\mathcal{H}^{\epsilon}$
and $\operatorname{Dom}(Q_{\epsilon})\subseteq\mathcal{H}_{\epsilon}$, respectively.
Let $Q$ be a non-negative closed quadratic form with domain $\operatorname{Dom}(Q)\subseteq\mathcal{H}$.
We assume that $Q$, $Q^{\epsilon}$ and $Q_{\epsilon}$ satisfy the
following assumptions:
\begin{itemize}
\item [(A11)] For all sufficiently small $\epsilon > 0$, we have

\begin{itemize}
\item [(i)] $\operatorname{Dom}(Q^{\epsilon})$ is dense in $\mathcal{H}^{\epsilon}$,
\item [(ii)] $\operatorname{Dom}(Q_{\epsilon})$ is dense in $\mathcal{H}_{\epsilon}$,
\item [(iii)] $\operatorname{Dom}(Q)$ is dense in $\mathcal{H}$.
\end{itemize}
\item [(A12)] For $0<\epsilon_2\leq\epsilon_1$ we have

\begin{itemize}
\item [(i)] $P_{\mathcal{H}^{\epsilon_1}, \mathcal{H}^{\epsilon_2}}(\operatorname{Dom}(Q^{\epsilon_1}))=\operatorname{Dom}(Q^{\epsilon_2})$,
\item [(ii)] $P_{\mathcal{H}^{\epsilon_1}, \mathcal{H}}(\operatorname{Dom}(Q^{\epsilon_1}))=\operatorname{Dom}(Q)$.
\end{itemize}
\item [(A13)] If $\epsilon_1>0$, then, for all sufficiently small
$\epsilon>0$, we have \[
P_{\mathcal{H}^{\epsilon_1}, \mathcal{H}_{\epsilon}}(\operatorname{Dom}(Q^{\epsilon_1}))=\operatorname{Dom}(Q_{\epsilon}).\]

\item [{(A14)}] For $0<\epsilon_2\leq\epsilon_1$ we have

\begin{itemize}
\item [{(i)}] $P_{\mathcal{H}_{\epsilon_2,}\mathcal{H}_{\epsilon_1}}(\operatorname{Dom}(Q_{\epsilon_2}))=\operatorname{Dom}(Q_{\epsilon_1})$,
\item [{(ii)}] $P_{\mathcal{H}, \mathcal{H}_{\epsilon_1}}(\operatorname{Dom}(Q))=\operatorname{Dom}(Q_{\epsilon_1})$.
\end{itemize}
\end{itemize}

\begin{definition}\label{def:2.2} \rm
Let $\epsilon_0>0$ be fixed.
For $0<\epsilon\leq\epsilon_0$ let $\hat{Q}^{\epsilon}$ be the
quadratic form with domain
\[
\operatorname{Dom}(\hat{Q}^{\epsilon})=\operatorname{Dom}(Q^{\epsilon})\oplus
(\mathcal{H}^{\epsilon})^{\bot}\mathcal{H}^{\epsilon_0}
\]
 and, if $f,g\in\operatorname{Dom}(Q^{\epsilon})$ and $h,i\in(\mathcal{H}^{\epsilon})^{\bot}\mathcal{H}^{\epsilon_0}$,
we define $\hat{Q}^{\epsilon}(f\oplus h,g\oplus i)$ by
\[
\hat{Q}^{\epsilon}(f+h,g+i)  =Q^{\epsilon}(f,g)
  =Q^{\epsilon}(P_{\mathcal{H}^{\epsilon_0},
 \mathcal{H}^{\epsilon}}(f+h),P_{\mathcal{H}^{\epsilon_0},
 \mathcal{H}^{\epsilon}}(g+i)).
\]
 \end{definition}

 Similarly we write $\hat{Q}$ and $\hat{Q}_{\epsilon}$ for the
quadratic forms with domains
\begin{gather*}
\operatorname{Dom}(\hat{Q}) =\operatorname{Dom}(Q)\oplus\mathcal{H}^{\bot}\mathcal{H}^{\epsilon_0},\\
\operatorname{Dom}(\hat{Q}_{\epsilon})
=\operatorname{Dom}(Q)\oplus(\mathcal{H}_{\epsilon})^{\bot}\mathcal{H}^{\epsilon_0},
\end{gather*}
 respectively, and, for all $f,g\in\mathcal{H}^{\epsilon_0}$, we
define $\hat{Q}(f,g)$ and $\hat{Q}_{\epsilon}(f,g)$ by
\begin{gather*}
\hat{Q}(f,g) =Q(P_{\mathcal{H}^{\epsilon_0}, \mathcal{H}}\,
f,P_{\mathcal{H}^{\epsilon_0},\mathcal{H}}\, g),\\
\hat{Q}_{\epsilon}(f,g)
=Q_{\epsilon}(P_{\mathcal{H}^{\epsilon_0},
\mathcal{H}_{\epsilon}}f,P_{\mathcal{H}^{\epsilon_0},
\mathcal{H}_{\epsilon}}g),
\end{gather*}
respectively. We assume that these quadratic forms satisfy
the following assumptions:
\begin{itemize}
\item [{(A15)}] If $0<\epsilon_2\leq\epsilon_1\leq\epsilon_0$, then,
for all $f\in\mathcal{H}^{\epsilon_1}$, we have

\begin{itemize}
\item [{(i)}] $Q^{\epsilon_1}(f,f)\geq Q^{\epsilon_2}(P_{\mathcal{H}^{\epsilon_1}, \mathcal{H}^{\epsilon_2}}f, P_{\mathcal{H}^{\epsilon_1}, \mathcal{H}^{\epsilon_2}}f)$,
\item [{(ii)}] $Q^{\epsilon_1}(f,f)\geq Q(P_{\mathcal{H}^{\epsilon_1}, \mathcal{H}}\, f, P_{\mathcal{H}^{\epsilon_1}, \mathcal{H}}\, f)$.
\end{itemize}
\item [{(A16)}] For all $\epsilon_1,\epsilon_2\in(0,\epsilon_0]$
and all $f\in\mathcal{H}^{\epsilon_1}$, we have \[\
Q^{\epsilon_1}(f,f)\geq
Q_{\epsilon_2}(P_{\mathcal{H}^{\epsilon_1},
\mathcal{H}_{\epsilon_2}}f,
P_{\mathcal{H}^{\epsilon_1},\mathcal{H}_{\epsilon_2}}f).\]

\item [{(A17)}] If $0<\epsilon_2\leq\epsilon_1\leq\epsilon_0$, then,
for all $f\in\mathcal{H}_{\epsilon_2}$, we have \[
Q_{\epsilon_2}(f,f)\geq
Q_{\epsilon_1}(P_{\mathcal{H}_{\epsilon_2},
\mathcal{H}_{\epsilon_1}}f, P_{\mathcal{H}_{\epsilon_2},
\mathcal{H}_{\epsilon_1}}f).\]

\item [{(A18)}] For all $0<\epsilon\leq\epsilon_0$ and all
$f\in\mathcal{H}$,
we have
\[
Q(f,f)\geq Q_{\epsilon}(P_{\mathcal{H}, \mathcal{H}_{\epsilon}}f,
P_{\mathcal{H}, \mathcal{H}_{\epsilon}}f).
\]

\item [{(A19)}] For all $f\in\mathcal{H}$ we have
\[
Q(f,f)=\lim_{\epsilon\downarrow0}Q_{\epsilon}(P_{\mathcal{H},
\mathcal{H}_{\epsilon}}f, P_{\mathcal{H}, \mathcal{H}_{\epsilon}}f).
\]

\item [{(A20)}] For all $f\in\operatorname{Dom}(Q^{\epsilon_0})$ we have
\[
Q(P_{\mathcal{H}^{\epsilon_0},\mathcal{H}}\, f,
P_{\mathcal{H}^{\epsilon_0},\mathcal{H}}\,
f)=\lim_{\epsilon\downarrow0}Q^{\epsilon}(P_{\mathcal{H}^{\epsilon_0},
\mathcal{H}^{\epsilon}}f, P_{\mathcal{H}^{\epsilon_0},
\mathcal{H}^{\epsilon}}f).
\]
\end{itemize}

\begin{definition}\label{def:2.3} \rm
For $0<\epsilon\leq\epsilon_0$
let $H_{\epsilon}\geq0$ be the self-adjoint operator associated to
$Q_{\epsilon}$ with domain $D(H_{\epsilon})\subseteq\mathcal{H}_{\epsilon}$.
Similarly, let $H^{\epsilon}\geq0$ and $H\geq0$ be the self-adjoint
operators associated to $Q^{\epsilon}$ and $Q$, respectively, with
domains $D(H^{\epsilon})\subseteq\mathcal{H}^{\epsilon}$ and
$D(H)\subseteq\mathcal{H}$.
\end{definition}

 Assumptions (A11)--(A18) imply that we have an
increasing family of non-negative quadratic forms:
\begin{equation}
\dots\leq\hat{Q}_{\epsilon_1}\leq\dots\leq\hat{Q}_{\epsilon_2}\leq\dots\leq\hat{Q}\leq\dots\leq\hat{Q}^{\epsilon_3}\leq\dots\leq\hat{Q}^{\epsilon_4}\leq\dots\label{eq:2.1}\end{equation}
 where
 \begin{equation}
0<\epsilon_2\leq\epsilon_1\leq\epsilon_0\quad \text{and }\quad
0<\epsilon_3\leq\epsilon_4\leq\epsilon_0.\label{eq:2.2}
\end{equation}
So by \cite[Theorem 4.17]{D1} we have, for all $\lambda>0$,
\begin{align*}
\dots & \geq(\lambda+H_{\epsilon_1})^{-1}\oplus\lambda^{-1}
 \geq\dots\geq(\lambda+H_{\epsilon_2})^{-1}\oplus\lambda^{-1}\geq\dots\\
\dots & \geq(\lambda+H)^{-1}\oplus\lambda^{-1}\geq\dots
 \geq(\lambda+H^{\epsilon_3})^{-1}\oplus\lambda^{-1}\geq\dots\\
\dots & \geq(\lambda+H^{\epsilon_4})^{-1}\oplus\lambda^{-1}
 \geq\dots
\end{align*}
 if $\epsilon_1,\epsilon_2,\epsilon_3,\epsilon_4$ satisfy
\eqref{eq:2.2}, where
$(\lambda+H_{\epsilon_1})^{-1}\oplus\lambda^{-1}$ is the
operator defined on
$\mathcal{H}^{\epsilon_0}=\mathcal{H}_{\epsilon_1}
\oplus(\mathcal{H}_{\epsilon_1})^{\bot}\mathcal{H}^{\epsilon_0}$
by
\[
[(\lambda+H_{\epsilon_1})^{-1}\oplus\lambda^{-1}](f+g)
=(\lambda+H_{\epsilon_1})^{-1}f+\lambda^{-1}g
\]
 for all $f\in\mathcal{H}_{\epsilon_1}$ and all
$g\in(\mathcal{H}_{\epsilon_1})^{\bot}\mathcal{H}^{\epsilon_0}$.
Similarly the operators $(\lambda+H)^{-1}\oplus\lambda^{-1}$ and
$(\lambda+H^{\epsilon})^{-1}\oplus\lambda^{-1}$ are defined on
$\mathcal{H}^{\epsilon_0}=\mathcal{H}\oplus\mathcal{H}^{\bot}
\mathcal{H}^{\epsilon_0}$
and
$\mathcal{H}^{\epsilon_0}=\mathcal{H}^{\epsilon}\oplus
(\mathcal{H}^{\epsilon})^{\bot}\mathcal{H}^{\epsilon_0}$,
respectively.

 For $0<\epsilon\leq\epsilon_0$ let $Q(\epsilon)$ be a
closed non-negative quadratic form with domain
$\operatorname{Dom}(Q(\epsilon))\subseteq\mathcal{A}(\epsilon)$ satisfying the
following assumptions:
\begin{itemize}
\item [{(A21)}] $\operatorname{Dom}(Q(\epsilon))$ is dense in $\mathcal{A}(\epsilon)$.
\item [{(A22)}] For $0<\epsilon\leq\epsilon_0$ we have

\begin{itemize}
\item [{(i)}] $P_{\mathcal{H}^{\epsilon}, \mathcal{A}(\epsilon)}(\operatorname{Dom}(Q^{\epsilon}))=\operatorname{Dom}(Q(\epsilon))$,
\item [{(ii)}] $P_{\mathcal{A}(\epsilon), \mathcal{H}_{\epsilon}}(\operatorname{Dom}(Q(\epsilon)))=\operatorname{Dom}(Q_{\epsilon})$.
\end{itemize}
\item[(A23)] If $0<\epsilon\leq\epsilon_0$, then, for all
$f\in\mathcal{H}^{\epsilon}$, we have\[
Q^{\epsilon}(f,f)\geq Q(\epsilon)(P_{\mathcal{H}^{\epsilon}, \mathcal{A}(\epsilon)}f,P_{\mathcal{H}^{\epsilon}, \mathcal{A}(\epsilon)}f),\]
and, for all $g\in\mathcal{A}(\epsilon)$, we have\[
Q(\epsilon)(g,g)\geq Q_{\epsilon}(P_{\mathcal{A}(\epsilon), \mathcal{H}_{\epsilon}}g,P_{\mathcal{A}(\epsilon), \mathcal{H}_{\epsilon}}g).\]
\end{itemize}

\begin{definition}\label{def:2.4} \rm
For $0<\epsilon\leq\epsilon_0$
we define the quadratic form $\hat{Q}(\epsilon)$, with domain
\[
\operatorname{Dom}(\hat{Q}(\epsilon))=\operatorname{Dom}(Q(\epsilon))\oplus\mathcal{A}
(\epsilon)^{\bot}\mathcal{H}^{\epsilon_0}
\subseteq\mathcal{H}^{\epsilon_0}
\]
by
\[
\hat{Q}(\epsilon)(f,g)=Q(\epsilon)(P_{\mathcal{H}^{\epsilon_0},
\mathcal{A}(\epsilon)}f,P_{\mathcal{H}^{\epsilon_0},
\mathcal{A}(\epsilon)}g)
\]
 for all $f,g\in\mathcal{H}^{\epsilon_0}$. We let $H(\epsilon)\geq0$
be the self-adjoint operator associated to $Q(\epsilon)$ with domain
$D(H(\epsilon))\subseteq\mathcal{A}(\epsilon)$.
\end{definition}

Assumption (A23) implies that if $0<\epsilon \leq \epsilon_0$, then
\begin{equation}\label{eq:2.3}
\hat{Q}_\epsilon \leq \hat{Q}(\epsilon)\leq \hat{Q}^\epsilon
\end{equation}
and hence, by \cite[Theorem 4.17]{D1},
\begin{equation}\label{eq:2.4}
(\lambda +H_\epsilon )^{-1}\oplus \lambda^{-1} \geq (\lambda
+H (\epsilon ))^{-1} \oplus \lambda^{-1} \geq (\lambda
+H^\epsilon )^{-1}\oplus \lambda ^{-1}
\end{equation}
for all $\lambda >0$, where $(\lambda +H(\epsilon ))^{-1}
\oplus \lambda^{-1}$ is the operator defined on
$\mathcal{H}^{\epsilon_0}=\mathcal{A}(\epsilon) \oplus
\mathcal{A}(\epsilon)^\bot \mathcal{H}^{\epsilon_0}$ by
\[
((\lambda +H(\epsilon ))^{-1}\oplus \lambda^{-1})(f+g)
=(\lambda +H(\epsilon))^{-1} f+\lambda^{-1}g
\]
for all $f\in \mathcal{A}(\epsilon)$ and
$g\in \mathcal{A}(\epsilon )^\bot \mathcal{H}^{\epsilon_0}$.

\begin{proposition}[{\cite[Theorem 4.32]{D1}}] \label{prop:2.5}
Let $K _n\geq 0$ be an increasing sequence of non-negative
self-adjoint operators with domains in a Hilbert space
$\mathcal{U}$. Put
\[
\mathcal{E}=\cap_n D(K^{1/2}_n)
\]
and let $\hat{\mathcal{U}}$ be the closure of $\mathcal{E}$.
Then there exists a self-adjoint operator $K\geq 0$ with
domain $D(K)\subseteq \hat{\mathcal{U}}$ such that its
associated quadratic form domain equal  $\mathcal{E}$ and that
\[
\langle K^{1/2} f,K^{1/2} f\rangle
= \lim_{n\to \infty} \langle K^{1/2} _n f,
K^{1/2} _n f\rangle \quad (f\in \mathcal{E}).
\]
Moreover
\[
\lim_{n\to \infty} \{ \sup_{0\leq t\leq a} \| e^{-K_nt} f-e^{-Kt}
f\| \} =0
\]
for all $a\geq 0$ and $f\in \hat{\mathcal{U}}$.
Hence for all $\lambda >0$ we have
\[
\| (\lambda +K_n)^{-1} f-(\lambda +K)^{-1} f\| \to 0
\quad \text{as } n\to \infty
\]
for all $f\in \hat{\mathcal{U}}$.
\end{proposition}

\begin{definition}\label{def:2.6} \rm
For $0<\epsilon \leq \epsilon_0$ we let $\hat{H}_{\epsilon} $
and $\hat{H}^\epsilon$ be the operators with domains
$D(\hat{H}_\epsilon )=D(H_\epsilon )\oplus
(\mathcal{H}_\epsilon )^\bot \mathcal{H}^{\epsilon_0}$ and
$D(\hat{H}^\epsilon)=D(H^\epsilon )\oplus (\mathcal{H}^\epsilon )^\bot
 \mathcal{H}^{\epsilon_0}$, respectively, defined by
\[
\hat{H}_\epsilon (f+g)=H_\epsilon f
=H_\epsilon P_{\mathcal{H}^{\epsilon_0} ,
\mathcal{H}_\epsilon }(f+g)
\]
for all $f+g\in D(H_\epsilon )\oplus (\mathcal{H}_\epsilon )^\bot
\mathcal{H}^{\epsilon _0}$, and
\[
\hat{H}^\epsilon (f+g) =H^\epsilon f=H^\epsilon
P_{\mathcal{H}^{\epsilon _0}, \mathcal{H}^\epsilon }(f+g)
\]
for all $f+ g\in D(H^\epsilon )\oplus (\mathcal{H}^\epsilon )^\bot
\mathcal{H}^{\epsilon_0}$. Similarly we write $\hat{H}$ to
denote the operator with domain
$D(\hat{H})=D(H)\oplus \mathcal{H}^\bot \mathcal{H}^{\epsilon_0}$
defined by
\[
\hat{H} (f+g) =\hat{H} f=\hat{H} P_{\mathcal{H}^{\epsilon _0} ,
\mathcal{H}} \,(f+g)
\]
for all $f+g\in D(H)\oplus \mathcal{H}^\bot \mathcal{H}^{\epsilon_0}$.
\end{definition}

 We also write $\hat{\hat{H}}_\epsilon$ for the operator with domain
$D(\hat{\hat{H}}_\epsilon )=D(H_\epsilon )\oplus
(\mathcal{H}_\epsilon) ^\bot \mathcal{H}$ defined by
\[
\hat{\hat{H}}_\epsilon (f+g)=H_\epsilon f=H_\epsilon P_{\mathcal{H},
\mathcal{H}_\epsilon }(f+g)
\]
for all $f+g\in D(H_\epsilon )\oplus (\mathcal{H}_\epsilon )^\bot
\mathcal{H}$.

\begin{lemma}\label{lem:2.7}
We have
\begin{enumerate}
\item[(i)] $\lim_{\epsilon \downarrow 0} \{ \sup_{0\leq t\leq a}
\| e^{-\hat{\hat{H}}_\epsilon t} f-e^{-Ht}f\| _{\mathcal{H}}\}=0$
for all $f\in \mathcal{H}$ and $a\geq 0$. Also
\[
\lim_{\epsilon \downarrow 0} \| (\lambda +\hat{\hat{H}}_\epsilon )^{-1}
f-(\lambda +H)^{-1} f\| _{\mathcal{H}}=0
\]
for all $f\in \mathcal{H}$ and $a\geq 0$.

\item[(ii)] $\lim_{\epsilon \downarrow 0}
\{ \sup_{0\leq t\leq a} \| e^{-\hat{H}_\epsilon t} f
-e^{-\hat{H}t} f\| _{\mathcal{H}^{\epsilon_0}}\}=0$
for all $f\in \mathcal{H}^{\epsilon_0}$ and $a\geq 0$.
Also
\[
\lim_{\epsilon\downarrow 0} \| (\lambda +\hat{H}_\epsilon ) ^{-1}
f-(\lambda +\hat{H})^{-1} f\| _{\mathcal{H}^{\epsilon_0}}=0
\]
for all $f\in \mathcal{H}^{\epsilon_0}$ and $\lambda >0$.
\end{enumerate}
\end{lemma}

\begin{proof} To prove (i) we apply Proposition \ref{prop:2.5} with
$\mathcal{U}=\mathcal{H}$,
$K_n = \hat{\hat{\mathcal{H_\varepsilon}}}$ and then use Assumptions
(A17), (A18) and (A19). Similarly, to prove (ii) we apply Proposition 2.5
with $\mathcal{U}=\mathcal{H}^{\epsilon_0}$ and $K_n =
\hat{\mathcal{H_\varepsilon}}$, and then use Assumptions (A17),
(A18) and (A19).
\end{proof}


\begin{definition}\label{def:2.8}\rm
 Let $\mathcal{U}$ be a Hilbert space and let $Q\geq 0$ be a closed
quadratic form  with domain $\operatorname{Dom} (Q)\subseteq \mathcal{U}$.
(Note that $\operatorname{Dom} (Q)$ is not necessarily dense in $\mathcal{U}$.)
 Let $H\geq 0$ be the self-adjoint operator associated to $Q$ with
domain $D(H)\subseteq \overline{\operatorname{Dom} (Q)}$.
If $\phi :\mathbb{R}\to \mathbb{R}$ is a bounded measurable function,
then we define the bounded operator $\phi (H)$ on
$\mathcal{U}=\overline{\operatorname{Dom} (Q)} \oplus ((\overline{\operatorname{Dom} (Q)})^\bot
\mathcal{U})$ by
\begin{equation}\label{eq:2.5}
\phi (Q) (f+g)=\phi (H)f=\phi (H)(P_{\mathcal{U},
 \overline{\operatorname{Dom} (Q)}}  (f+g))\end{equation}
for all $f\in \overline{\operatorname{Dom} (Q)}$ and $g\in
(\overline{\operatorname{Dom}(Q)})^\bot \mathcal{U}$.
\end{definition}

Similarly, on $\mathcal{U}=\overline{\operatorname{Dom} (Q)} \oplus
((\overline{\operatorname{Dom} (Q)})^\bot \mathcal{U})$,
we define the bounded operator $[\phi (Q)]_M$ by
\begin{equation} \label{eq:2.6}
\begin{split}
[\phi (Q)]_M(f+g)&= \phi (H)f+g\\
&=\phi (H)P_{\mathcal{U},  \overline{\operatorname{Dom} (Q)}}\,(f+g)
 +P_{\mathcal{U}, \overline{(\operatorname{Dom} (Q))}^\bot \mathcal{U}}(f+g)
\end{split}
\end{equation}
for all $f\in \overline{\operatorname{Dom} (Q)}$ and
$g\in (\overline{\operatorname{Dom} (Q)})^\bot \mathcal{U}$.

In both \eqref{eq:2.5} and \eqref{eq:2.6}, $\phi (H)$ is
the bounded operator on $\overline{\operatorname{Dom} (Q)}$ defined using
the spectral theorem.

\begin{definition}\label{def:2.9} \rm
Let $\mathcal{U}$ be a Hilbert space and for $n=1,2,3,\dots$
let $Q_n\geq 0$ be a closed quadratic form with domain
$\operatorname{Dom} (Q_n)\subseteq \mathcal{U}$. ($\operatorname{Dom} (Q_n)$ is not necessarily
dense in $\mathcal{U}$.) Let $Q\geq 0$ be a closed quadratic form
with domain in $\mathcal{U}$. ($\operatorname{Dom} (Q)$ is not necessarily
dense in $\mathcal{U}$.) We say that $Q_n$ converges to $Q$ in the
strong resolvent sense $(\operatorname{srs} )$ if for some $\lambda >0$ we have
\[
\lim_{n\to \infty} (\lambda+Q_n)^{-1}f=(\lambda +Q)^{-1}f\quad
(f\in \mathcal{U}).
\]
\end{definition}

\begin{lemma}\label{lem:2.10}
Let $\mathcal{U}$, $Q_n$ and $Q$ be as in Definitions~\ref{def:2.8}
and \ref{def:2.9}. Let $P_n$ be the orthogonal projection of
$\mathcal{U}$ onto $\overline{\operatorname{Dom} (Q_n)}$. Suppose that for all
$f\in \mathcal{U}$ we have
\[
\| P_n f-f\| \to 0 \quad \text{as } n\to \infty.
\]
Suppose also that $\overline{\operatorname{Dom} (Q)}=\mathcal{U}$. Then
$Q_n\overset{\operatorname{srs}}{\longrightarrow} Q$ as $n\to \infty$ is
equivalent to
\[
[(\lambda +Q_n)^{-1} ]_M \,f\to [(\lambda +Q)^{-1}]_M f \quad
\text{as } n\to \infty
\]
for some $\lambda >0$ and for all $f\in \mathcal{U}$.
\end{lemma}

 The proof of this lemma is obvious.

\begin{proposition}[{\cite[Theorem~1.2.3]{D2}}]\label{prop:2.11}
Let $K_n\geq 0$, $n=1,2,3,\dots $, and $K\geq 0$ be self-adjoint
 operators with domains in a Hilbert space $\mathcal{U}$.
Suppose that
\[
K_1\geq K_2 \geq \dots \geq K_n \geq K_{n+1}\geq \dots
\geq K
\]
and that their associated quadratic forms satisfy
\[
\langle K^{1/2} f, K^{1/2} f\rangle
=\lim_{n\to \infty} \langle K^{1/2}_n f,
K^{1/2}_n f\rangle
\]
for all $f$ in a form core of $K$. Then $K_n$ converges to $K$
in the strong resolvent sense.
\end{proposition}

\begin{definition}\label{def:2.12} \rm
We let $\mathcal{C}$ be the subspace of $\operatorname{Dom} (\hat{Q})$ defined by
\[
\mathcal{C}=\cup_{0<\epsilon \leq \epsilon_0}
\operatorname{Dom} (Q^\epsilon )\oplus (\mathcal{H}^\epsilon )^\bot
 \mathcal{H}^{\epsilon_0}.\]
(Note that $\mathcal{C}$ is a subspace of $\operatorname{Dom} (\hat{Q})$
by Assumption~(A15).)
\end{definition}

\begin{lemma}\label{lem:2.13}
$\mathcal{C}$ is a form core of $\hat{Q}$.
\end{lemma}

\begin{proof}
We first recall that, by Assumption~(A12),
\[
\operatorname{Dom} (Q)=P_{\mathcal{H}^\epsilon , \mathcal{H}}
(\operatorname{Dom} (Q^\epsilon ))\quad (0<\epsilon \leq \epsilon_0).
\]
Let $f=g+h\in \operatorname{Dom} (\hat{Q})$, where $g\in \operatorname{Dom} (Q)$ and
$h\in \mathcal{H}^\bot \mathcal{H}^{\epsilon_0}$.
Let $\alpha \in \operatorname{Dom} (Q^{\epsilon_0})$ such that
\[
P_{\mathcal{H}^{\epsilon_0},\mathcal{H}}\alpha =g.
\]
For $0<\epsilon \leq \epsilon_0$ let
\begin{align*}
g_\epsilon &=P_{\mathcal{H}^{\epsilon_0}, \mathcal{H}^\epsilon}\alpha =P_{\mathcal{H}^\epsilon , \mathcal{H}}\, g_\epsilon +P_{\mathcal{H}^\epsilon , \mathcal{H}^\bot \mathcal{H}^\epsilon} g_\epsilon\\
&=P_{\mathcal{H}^{\epsilon_0},\mathcal{H}}  \alpha
+P_{\mathcal{H}^\epsilon ,\mathcal{H}^\bot \mathcal{H}^\epsilon} g_\epsilon \\
&=g+P_{\mathcal{H}^\epsilon , \mathcal{H}^\bot
\mathcal{H}^\epsilon} g_\epsilon
\end{align*}
and let
\[
h_\epsilon =P_{\mathcal{H}^\bot \mathcal{H}^{\epsilon_0} ,
(\mathcal{H}^\epsilon )^\bot \mathcal{H}^{\epsilon _0}} h
\]
and let
\begin{equation} \label{eq:2.7}
\begin{split}
f_\epsilon
&= g_\epsilon +h_\epsilon \\
&= P_{\mathcal{H}^{\epsilon_0}, \mathcal{H}} \alpha
 +P_{\mathcal{H}^\epsilon ,\mathcal{H}^\bot \mathcal{H}^\epsilon }
g_\epsilon +h_\epsilon \\
&= g+P_{\mathcal{H}^\epsilon ,\mathcal{H}^\bot \mathcal{H}^\epsilon }
g_\epsilon +h_\epsilon .
\end{split}
\end{equation}
Then, by (A12), $f_\epsilon \in \operatorname{Dom}  (Q^\epsilon )\oplus
(\mathcal{H}^\epsilon )^\bot \mathcal{H}^{\epsilon_0}$. Since
\begin{align*}
 h&=P_{\mathcal{H}^\bot \mathcal{H}^{\epsilon_0} ,(\mathcal{H}^\epsilon )^\bot \mathcal{H}^{\epsilon_0}} h+ (I_{\mathcal{H}^\bot \mathcal{H}^{\epsilon_0}} -P_{\mathcal{H}^\bot \mathcal{H}^{\epsilon_0}, \,(\mathcal{H}^\epsilon )^\bot \mathcal{H}^{\epsilon_0}} )h\\
&= h_\epsilon +(I_{\mathcal{H}^\bot \mathcal{H}^{\epsilon_0}}
-P_{\mathcal{H}^\bot \mathcal{H}^{\epsilon_0} ,
(\mathcal{H}^\epsilon)^\bot \mathcal{H}^{\epsilon _0}})h,
\end{align*}
we have
\begin{equation} \label{eq:2.8}
\begin{split}
f-f_\epsilon
&= g+h-(g+P_{\mathcal{H}^\epsilon , \mathcal{H}^\bot \mathcal{H}^\epsilon} g_\epsilon +h_\epsilon )\\
&=g+h_\epsilon +(I_{\mathcal{H}^\bot \mathcal{H}^{\epsilon _0}}
 -P_{\mathcal{H}^\bot \mathcal{H}^{\epsilon_0} ,
 (\mathcal{H}^\epsilon)^\bot \mathcal{H}^{\epsilon_0}})h
 - (g+P_{\mathcal{H}^\epsilon , \mathcal{H}^\bot \mathcal{H}^\epsilon} g_\epsilon +h_\epsilon )\\
&= (I_{\mathcal{H}^\bot \mathcal{H}^{\epsilon_0}} -P_{\mathcal{H}^\bot \mathcal{H}^{\epsilon_0},  (\mathcal{H}^\epsilon )^\bot \mathcal{H}^{\epsilon_0}} )h-P_{\mathcal{H}^\epsilon , \mathcal{H}^\bot \mathcal{H}^\epsilon} g_\epsilon\\
&= (I_{\mathcal{H}^\bot \mathcal{H}^{\epsilon_0}}-P_{\mathcal{H}^\bot \mathcal{H}^{\epsilon_0}, (\mathcal{H}^\epsilon )^\bot \mathcal{H}^{\epsilon_0}})h-P_{\mathcal{H}^{\epsilon_0}, \mathcal{H}^\bot \mathcal{H}^\epsilon} \alpha\\
&=(I_{\mathcal{H}^\epsilon} -P_{\mathcal{H}^\epsilon , \mathcal{H}} )P_{\mathcal{H}^{\epsilon_0}, \mathcal{H}^\epsilon } h
 - (I_{\mathcal{H}^\epsilon } -P_{\mathcal{H}^\epsilon , \mathcal{H} } )P_{\mathcal{H}^{\epsilon_0} , \mathcal{H}^\epsilon } \alpha\\
& \to 0 \quad  \text{as }  \epsilon \downarrow 0 \quad   \text{(by (A5))}.\end{split}\end{equation}
Also, by~\eqref{eq:2.8},
\begin{align*}
\hat{Q} (f-f_\epsilon ,f-f_\epsilon )
&=\hat{Q} (P_{\mathcal{H}^\epsilon, \, \mathcal{H}^\bot
\mathcal{H}^\epsilon} P_{\mathcal{H}^{\epsilon_0} ,
 \mathcal{H}^\epsilon} (h-\alpha),
 P_{\mathcal{H}^\epsilon , \mathcal{H}^\bot
\mathcal{H}^\epsilon} P_{\mathcal{H}^{\epsilon_0} ,
\mathcal{H}^\epsilon} (h-\alpha ))\\
&=0
\end{align*}
since $P_{\mathcal{H}^\epsilon , \mathcal{H}^\bot
\mathcal{H}^\epsilon } P_{\mathcal{H}^{\epsilon _0} ,
\mathcal{H}^\epsilon} (h-\alpha )\in \mathcal{H}^\bot
\mathcal{H}^{\epsilon_0}$. Also, by Assumption~(A12),
it is not difficult to show that $\mathcal{C}$ is closed
under addition and scalar multiplication. Hence $\mathcal{C}$
is a form core of $\hat{Q}$.
\end{proof}

\begin{theorem}\label{thm:2.14}
We have $\hat{H}^\epsilon 
\overset{\operatorname{srs}}{\longrightarrow} \hat{H}$
 as $\epsilon \downarrow 0$.
\end{theorem}

\begin{proof}
Let $\delta \in (0,\epsilon _0]$ and let
$f\in \operatorname{Dom} (Q^\delta )\oplus (\mathcal{H}^{\delta})^\bot
\mathcal{H}^{\epsilon_0}$. Then, for $0<\epsilon<\delta$,
we have, by (A5),
\[
P_{\mathcal{H}^{\epsilon_0} , \mathcal{H}^\epsilon} f
=P_{\mathcal{H}^{\epsilon_0} , \mathcal{H}^\epsilon }f
-P_{\mathcal{H}^{\epsilon_0} ,\mathcal{H}}
  f+P_{\mathcal{H}^{\epsilon_0} ,\mathcal{H}} f
\to P_{\mathcal{H}^{\epsilon_0} , \mathcal{H} }
f \quad \text{as } \epsilon\downarrow 0.
\]
Hence, for $0<\epsilon <\delta$, we have, by (A20),
\begin{align*}
\hat{Q}^\epsilon (f,f)&= Q^\epsilon (P_{\mathcal{H}^{\epsilon_0} ,
\mathcal{H}^\epsilon } f,P_{\mathcal{H}^{\epsilon_0} ,
\mathcal{H}^\epsilon } f)\\
&\to Q(P_{\mathcal{H}^{\epsilon_0} ,\mathcal{H}}
 f,P_{\mathcal{H}^{\epsilon_0} ,\mathcal{H} }  f)
= \hat{Q} (f,f)\quad \text{as } \epsilon \downarrow 0.
\end{align*}
Thus for all $f\in \mathcal{C}$ we have
\begin{equation}\label{eq:2.9}
\hat{Q}(f,f)=\lim_{\epsilon \downarrow 0} \hat{Q}^\epsilon (f,f).
\end{equation}
The theorem now follows from Proposition~\ref{prop:2.11}
together with \eqref{eq:2.1}, \eqref{eq:2.9} and
Lemma~\ref{lem:2.13}.
\end{proof}

\begin{definition}\label{def:2.15} \rm
 For $0<\epsilon \leq \epsilon_0$ we let $\hat{H}(\epsilon )$
be the operator with domain
$D(\hat{H}(\epsilon ))=D(H(\epsilon ))\oplus \mathcal{A}
(\epsilon )^\bot \mathcal{H}^{\epsilon _0}$
defined by
\[
\hat{H} (\epsilon )(f+g)=H(\epsilon )f
=H(\epsilon )P_{\mathcal{H}^{\epsilon_0} ,
\mathcal{A}(\epsilon)} (f+g)
\]
for all $f\in D(H(\epsilon))$ and $g \in \mathcal{A}(\epsilon )^\bot
\mathcal{H}^{\epsilon_0}$. Thus $\hat{H}(\epsilon )\geq 0$
is the self-adjoint operator associated to the quadratic form
$\hat{Q}(\epsilon )$ defined in Definition~\ref{def:2.4}.
By \eqref{eq:2.4} we have
\[
(\lambda +\hat{H}_\epsilon )^{-1}
\geq (\lambda +\hat{H}(\epsilon ))^{-1}\geq (\lambda
+\hat{H}^\epsilon )^{-1}
\]
for all $\lambda >0$ and $0<\epsilon \leq \epsilon _0$; i.e.,
\begin{equation}\label{eq:2.10}
\langle (\lambda +\hat{H}_\epsilon )^{-1} f,
f\rangle \geq \langle (\lambda +\hat{H}(\epsilon ))^{-1} f,
f\rangle \geq \langle (\lambda +\hat{H}^\epsilon )^{-1} f,
f\rangle
\end{equation}
for all $f\in \mathcal{H}^{\epsilon _0}$, $\lambda >0$ and
$0<\epsilon \leq \epsilon _0$.
\end{definition}

\begin{lemma}\label{lem:2.16}
We have
\[
\langle (\lambda +\hat{H})^{-1} f,f\rangle
=\lim_{\epsilon \downarrow 0} \langle (\lambda
+\hat{H}(\epsilon ))^{-1} f,f\rangle
\]
for all $f\in \mathcal{H}^{\epsilon _0}$ and
$\lambda >0$.
\end{lemma}

\begin{proof} This lemma follows from the second inequality of
Lemma~\ref{lem:2.7}(ii), Theorem~\ref{thm:2.14} and \eqref{eq:2.10}.
\end{proof}

\begin{theorem}\label{thm:2.17}
For all $\lambda >0$ we have
\[
(\lambda +\hat{H})^{-1} f=\lim_{\epsilon\downarrow 0}
(\lambda+\hat{H}(\epsilon))^{-1} f
\]
for all $f\in \mathcal{H}^{\epsilon_0}$. Hence for all
$a>0$ and $f\in\mathcal{H}^{\epsilon_0}$ we have
\[
\lim_{\epsilon\downarrow 0} \{ \sup_{0\leq t\leq a}
\| e^{-\hat{H}(\epsilon )t} f-e ^{-\hat{H}t}
f\|_{\mathcal{H}^{\epsilon_0}} \} =0.
\]
\end{theorem}

\begin{proof}
By Lemma~\ref{lem:2.7}(ii), we have, for all $\lambda >0$,
\[
(\lambda +\hat{H})^{-1} f=\lim_{\epsilon\downarrow 0}
(\lambda +\hat{H}_\epsilon)^{-1} f\quad
(f\in \mathcal{H}^{\epsilon_0}).
\]
This is equivalent to having
\begin{equation}\label{eq:2.11}
\lim_{\epsilon \downarrow 0} \{ \sup_{0\leq t\leq a}
\| e^{-\hat{H}_\epsilon t} f-e^{-\hat{H} t}
f\| _{\mathcal{H}^{\epsilon_0}}\}=0\quad
(f\in \mathcal{H}^{\epsilon_0} )
\end{equation}
for all $a>0$ (see, for example \cite[Theorem 3.17]{D1}).
 Similarly, Theorem~\ref{thm:2.14} is equivalent to
\begin{equation}\label{eq:2.12}
\lim_{\epsilon\downarrow 0} \{\sup_{0\leq t\leq a}
\| e^{-\hat{H}^\epsilon t} f-e^{-\hat{H}t}
f\|_{\mathcal{H}^{\epsilon _0}} \}=0\quad
(f\in \mathcal{H}^{\epsilon_0})
\end{equation}
for all $a>0$. Since, for $\lambda >0$, we have
\begin{gather*}
(\lambda +\hat{H}_\epsilon )^{-1/2} f
=\int^\infty_0 \frac{1}{\sqrt{\pi t}}e^{-\lambda t}
 e^{-\hat{H}_\epsilon t} f\,dt\quad (f\in \mathcal{H}^{\epsilon_0}),\\
(\lambda+\hat{H}^\epsilon)^{-1/2} f
= \int^\infty_0 \frac{1}{\sqrt{\pi t}}
e^{-\lambda t} e^{-\hat{H}^\epsilon t} f\,dt \quad
(f\in \mathcal{H}^{\epsilon _0} ),
\end{gather*}
we have, from \eqref{eq:2.11} and \eqref{eq:2.12},
\begin{equation}\label{eq:2.13}
\lim_{\epsilon \downarrow 0} (\lambda
+\hat{H}_\epsilon )^{-1/2} f
=\lim_{\epsilon \downarrow 0 }(\lambda
+\hat{H}^\epsilon )^{-1/2} f
=(\lambda +\hat{H})^{-1/2}f
\end{equation}
for all $\lambda >0$ and $f\in \mathcal{H}^{\epsilon_0}$.
Since, for all $\lambda >0$,
\[
(\lambda +\hat{H}_\epsilon )^{-1} \geq
(\lambda +\hat{H}(\epsilon))^{-1}\geq (\lambda
+\hat{H}^\epsilon )^{-1},
\]
we have
\[
(\lambda +\hat{H}_\epsilon )^{-1/2}
\geq (\lambda +\hat{H}(\epsilon))^{-1/2}
\geq (\lambda +\hat{H}^\epsilon )^{-1/2}
\]
for all $\lambda >0$ (see, for example, \cite[Lemma 4.19]{D1});
 i.e., for all $0<\epsilon \leq \epsilon_0$, $\lambda >0$ and
$f\in \mathcal{H}^{\epsilon_0}$, we have
\begin{equation}\label{eq:2.14}
\langle (\lambda +\hat{H}_\epsilon )^{-1/2} f,f\rangle
\geq \langle (\lambda +\hat{H}(\epsilon ))^{-1/2} f,f\rangle
\geq \langle (\lambda +\hat{H}^\epsilon )^{-1/2} f,f\rangle.
\end{equation}
Hence, from \eqref{eq:2.13} and \eqref{eq:2.14}, we have
\begin{equation}\label{eq:2.15}
\langle (\lambda +\hat{H})^{-1/2} f,f\rangle
=\lim_{\epsilon \downarrow 0} \langle (\lambda +\hat{H}
(\epsilon ))^{-1/2} f,f \rangle
\end{equation}
for all $\lambda >0$ and $f\in \mathcal{H}^{\epsilon_0}$.
The polarization identity (see, for example, \cite[p.103]{D1})
and \eqref{eq:2.15} imply that
\begin{equation}\label{eq:2.16}
\langle (\lambda +\hat{H})^{-1/2} f,g\rangle
 =\lim_{\epsilon \downarrow 0} \langle
(\lambda +H(\epsilon ))^{-1/2} f,g\rangle
\end{equation}
for all $\lambda >0$ and $f,g\in \mathcal{H}^{\epsilon_0}$.
We now need the following result.

\begin{proposition}[{See \cite[Problem 4.11]{D1}}]
\label{prop:2.18}
Let $\mathcal{U}$ be a Hilbert space and let $f,f_n\in \mathcal{U}$ for  $n=1,2,3,\dots$. Suppose that
\[
 \langle f, g\rangle =\lim_{n\to \infty} \langle f_n, g\rangle
\quad (g\in \mathcal{U}).
\]
Then
\[
\lim_{n\to \infty} \| f_n-f\|=0\quad
\text{if and only if}\quad
\lim_{n\to \infty} \| f_n\|=\| f\|.
\]
\end{proposition}

 By Lemma~\ref{lem:2.16}, we have
\begin{equation}\label{eq:2.17}
 \lim_{\epsilon \downarrow 0} \| (\lambda +\hat{H}(\epsilon ))
^{-1/2} f\|_{\mathcal{H}^{\epsilon _0}}
=\| (\lambda +\hat{H})^{-1/2} f\| _{\mathcal{H}^{\epsilon _0}}
\end{equation}
for all $\lambda >0$ and $f\in \mathcal{H}^{\epsilon _0}$.
Proposition~\ref{prop:2.18} together with \eqref{eq:2.16}
and \eqref{eq:2.17} imply that
\begin{equation}\label{eq:2.18}
(\lambda +\hat{H})^{-1/2} f=\lim_{\epsilon \downarrow 0}
(\lambda +\hat{H}(\epsilon ))^{-1/2} f
\end{equation}
for all $\lambda >0$ and $f\in \mathcal{H}^{\epsilon_0}$. Hence
\begin{align*}
&(\lambda +\hat{H}(\epsilon ))^{-1} f-(\lambda +\hat{H})^{-1} f\\
 &= (\lambda +\hat{H}(\epsilon ))^{-1/2} [(\lambda +\hat{H}(\epsilon ))^{-1/2} f-(\lambda +\hat{H})^{-1/2} f]\\
&\quad + (\lambda +\hat{H}(\epsilon ))^{-1/2}
(\lambda +\hat{H})^{-1/2} f-(\lambda +\hat{H})^{-1/2}
(\lambda +\hat{H})^{-1/2} f
\to  0 \quad \text{as } \epsilon \downarrow 0
\end{align*}
for all $\lambda >0$ and $f\in \mathcal{H}^{\epsilon _0}$.
The strong convergence of $e^{-\hat{H}(\epsilon )t} $
to $e^{-\hat{H}t}$ now follows from \cite[Theorem 3.17]{D1}.
\end{proof}

 We next impose more assumptions on the operators $H$, $H^\epsilon $,
$H_\epsilon $ and  $H(\epsilon )$, $0<\epsilon \leq \epsilon_0$:
\begin{itemize}
\item[(A24)] $H$, $H^\epsilon $, $H_\epsilon$, $H(\epsilon )$,
$0<\epsilon \leq \epsilon_0$, have compact resolvents in the
Hilbert spaces $\mathcal{H}$, $\mathcal{H}^\epsilon $, $\mathcal{H}_\epsilon $
and $\mathcal{A}(\epsilon )$, respectively.

\item[(A25)] $0\in Sp (H)$, $0\in Sp (H^\epsilon )$,
$0\in Sp (H_\epsilon )$ and $0\in Sp (H(\epsilon ))$,
$0<\epsilon \leq \epsilon _0$.
\end{itemize}

\begin{definition}\label{def:2.19} \rm
We shall write $\{ \mu_i\}^\infty_{i=1}$ for the eigenvalues of $H$,
where $\{ \mu_i\}^\infty_{i=1}$ is a non-decreasing sequence and
the eigenvalues are listed repeatedly according to multiplicity.
Similarly, for $0<\epsilon \leq \epsilon _0$, we shall write
$\{ \mu^\epsilon _i\}^\infty_{i=1}$, $\{ \mu _{i,\epsilon }\}^\infty
 _{i=1}$, and
$\{ \mu_i (\epsilon )\}^\infty_{i=1}$ for the eigenvalues of
$H^\epsilon$, $H_\epsilon $ and $H(\epsilon )$, respectively.
Thus, by (A25), we have
\[
0=\mu_1=\mu^\epsilon _1 =\mu_{1,\epsilon }
=\mu_1 (\epsilon )\quad (0<\epsilon \leq \epsilon _0).
\]
We shall also write $\{ \varphi_i\}^\infty_{i=1}$,
$\{ \varphi^\epsilon _i\}^\infty_{i=1}$,
$\{\varphi_{i,\epsilon }\}^\infty_{i=1}$ and
$\{ \varphi_i(\epsilon)\}^\infty_{i=1}$ for the corresponding
normalized eigenvectors of $H$, $H^\epsilon$, $H_\epsilon$
and $H(\epsilon)$, respectively. We shall also assume that
$\{ \varphi_i\}^\infty_{i=1}$,
$\{ \varphi _i^\epsilon \}^\infty_{i=1}$,
$\{ \varphi_{i,\epsilon }\}^\infty_{i=1}$ and
$\{ \varphi_i(\epsilon )\}^\infty_{i=1}$ are complete
orthonormal systems in their respective Hilbert spaces
$\mathcal{H}$, $\mathcal{H}^\epsilon$, $\mathcal{H}_\epsilon$
and $\mathcal{H}(\epsilon )$.
\end{definition}

\begin{itemize}
\item[(A26)] $\mu_1$, $\mu_1^\epsilon$, $\mu_{1,\epsilon }$,
$\mu_1(\epsilon)$, $0<\epsilon \leq \epsilon_0$, all have
multiplicity $1$.

\item[(A27)] For $0<\epsilon \leq \epsilon_0$, we assume that
$P_{\mathcal{H}^{\epsilon_0}, \mathcal{H}}  \varphi^{\epsilon_0}_1$,
$P_{\mathcal{H}^{\epsilon_0}, \mathcal{H}^\epsilon} \varphi^{\epsilon_0}_1$, $P_{\mathcal{H}^{\epsilon_0}, \mathcal{H}_\epsilon}\varphi^{\epsilon_0}_1$ and $P_{\mathcal{H}^{\epsilon_0}, \mathcal{A}(\epsilon)} \varphi_1^{\epsilon_0}$ are eigenvectors of $H$, $H^\epsilon$, $H_\epsilon$ and $H(\epsilon)$, respectively, associated to the eigenvalue $0=\mu _1=
\mu_1^\epsilon =\mu_{1,\epsilon}=\mu_1(\epsilon)$.
In fact we assume that $\varphi_1$, $\varphi_1^\epsilon $,
$\varphi_{1,\epsilon}$ and $\varphi_1(\epsilon)$ are chosen so that
\begin{gather*}
\varphi_1
 =\| P_{\mathcal{H}^{\epsilon_0} ,\mathcal{H}}
 \varphi_1^{\epsilon _0} \|_\mathcal{H}^{-1}
P_{\mathcal{H}^{\epsilon_0}, \mathcal{H}} \varphi^{\epsilon_0}_1,\\
\varphi^\epsilon_1
= \|P_{\mathcal{H}^{\epsilon_0}, \mathcal{H}^\epsilon}
\varphi_1^{\epsilon _0} \|^{-1}_{\mathcal{H}^\epsilon} P_{\mathcal{H}^{\epsilon_0}, \mathcal{H}^\epsilon} \varphi_1^{\epsilon_0},\\
\varphi_{1,\epsilon }= \| P_{\mathcal{H}^{\epsilon_0} , \mathcal{H}_\epsilon} \varphi_1^{\epsilon_0} \| ^{-1}_{\mathcal{H}_\epsilon} P_{\mathcal{H}^{\epsilon_0}, \, \mathcal{H}_\epsilon} \varphi^{\epsilon_0}_1,\\
\varphi_1 (\epsilon)=\|P_{\mathcal{H}^{\epsilon_0},
\mathcal{A}(\epsilon)} \varphi_1^{\epsilon_0} \|^{-1}_{\mathcal{A}
(\epsilon)}P_{\mathcal{H}^{\epsilon_0} , \mathcal{A}(\epsilon)}
 \varphi_1^{\epsilon_0}.
\end{gather*}

\item[(A28)] For all $0<t\leq 1$ and $n=1,2,3,\dots$, we assume that
\begin{gather*}
\lim_{\epsilon \downarrow 0} \| P_{\mathcal{H},
\mathcal{B}(\epsilon )} e^{-Ht} \varphi_n -e^{-H(\epsilon )t}
P_{\mathcal{H},  \mathcal{B}(\epsilon)}
\varphi_n\|_{\mathcal{A}(\epsilon)}=0,\\
\lim_{\epsilon \downarrow 0} \| e^{-Ht} P_{\mathcal{A}(\epsilon ),
\mathcal{B}(\epsilon )} \varphi_n (\epsilon ) -P_{\mathcal{A}
(\epsilon ), \mathcal{B}(\epsilon )} e^{-H(\epsilon )t}
\varphi_n (\epsilon ) \|_{\mathcal{H}} =0,\\
\lim_{\epsilon \downarrow 0} \| P_{\mathcal{A}(\epsilon ),
\mathcal{B}(\epsilon )} \varphi_n (\epsilon )\|_{\mathcal{H}}
=1.
\end{gather*}
\end{itemize}

\begin{theorem}\label{thm:2.20} We have
$\lim_{\epsilon \downarrow 0} \mu_2 (\epsilon )=\mu_2$.
\end{theorem}

\begin{proof}
For $0<\epsilon\leq \epsilon _0$ let
\begin{equation} \label{eq:2.19} \beta_1 (\epsilon )
=\langle P_{\mathcal{H}, \mathcal{B}(\epsilon)} \varphi_2 ,
\varphi_1 (\epsilon )\rangle _{\mathcal{A}(\epsilon )}.
\end{equation}
Then
\begin{equation}\begin{split}\label{eq:2.20}
&e^{-\mu_2(\epsilon )t}\\
&\geq \| P_{\mathcal{H}, \mathcal{B}(\epsilon )} \varphi_2 -\beta_1 (\epsilon )\varphi_1 (\epsilon )\|^{-2}_{\mathcal{A}(\epsilon )}\\
&\quad \times \langle e ^{-H(\epsilon )t} (P_{\mathcal{H},\mathcal{B}(\epsilon )} \varphi_2 -\beta_1 (\epsilon )\varphi_1 (\epsilon )),
(P_{\mathcal{H}, \mathcal{B}(\epsilon )} \varphi_2 -\beta_1 (\epsilon ) \varphi_1 (\epsilon ))\rangle _{\mathcal{A} (\epsilon )}\\
&= \| P_{\mathcal{H}, \mathcal{B}(\epsilon )} \varphi_2
 -\beta_1 (\epsilon )\varphi_1 (\epsilon )
 \|^{-2}_{\mathcal{A}(\epsilon )}
 \{ \langle e^{-H(\epsilon )t} P_{\mathcal{H}, \mathcal{B}(\epsilon )}
 \varphi_2 ,P_{\mathcal{H}, \mathcal{B}(\epsilon )}\varphi_2
 \rangle _{\mathcal{A}(\epsilon )}\\
&\quad - 2\beta _1 (\epsilon )\langle e^{-H(\epsilon )t}
  P_{\mathcal{H}, \mathcal{B}(\epsilon )} \varphi_2 ,
 \varphi_1 (\epsilon )\rangle _{\mathcal{A}(\epsilon )}
 +\beta_1 (\epsilon )^2\}\\
&=\| P_{\mathcal{H}, \mathcal{B}(\epsilon )} \varphi_2
 -\beta_1 (\epsilon )\varphi_1 (\epsilon )\|^{-2}
 _{\mathcal{A}(\epsilon )}
 \{ \langle e^{-H(\epsilon )t}P_{\mathcal{H},
\mathcal{B}(\epsilon )} \varphi_2,
P_{\mathcal{H}, \mathcal{B}(\epsilon )}\varphi_2
\rangle_{\mathcal{A}(\epsilon )}\\
&\quad  -\beta _1 (\epsilon )^2\}.
\end{split}
\end{equation}

Consider the following term in \eqref{eq:2.20}:
\begin{align*}
&\langle e^{-H(\epsilon )t} P_{\mathcal{H}, \mathcal{B}(\epsilon )}\varphi_2, P_{\mathcal{H}, \mathcal{B}(\epsilon )} \varphi_2\rangle _{\mathcal{A} (\epsilon )}\\
&= \langle e ^{-H(\epsilon )t} P_{\mathcal{H}, \mathcal{B}(\epsilon )}\varphi_2 -P_{\mathcal{H}, \mathcal{B}(\epsilon )}e^{-Ht} \varphi_2, P_{\mathcal{H}, \mathcal{B}(\epsilon )} \varphi _2 \rangle _{\mathcal{A}(\epsilon )}\\
&\quad+\langle P_{\mathcal{H}, \mathcal{B}(\epsilon )} e ^{-Ht} \varphi_2 ,P_{\mathcal{H}, \mathcal{B}(\epsilon )} \varphi_2\rangle _{\mathcal{A}(\epsilon )}\\
&= \langle e^{-H(\epsilon )t} P_{\mathcal{H}, \mathcal{B}(\epsilon )} \varphi_2 -P_{\mathcal{H}, \, \mathcal{B}(\epsilon )} e^{-Ht} \varphi_2 ,P_{\mathcal{H}, \mathcal{B}(\epsilon )} \varphi_2\rangle _{\mathcal{A},(\epsilon )}\\
&\quad+ e^{-\mu_2 t} \langle P_{\mathcal{H}, \mathcal{B}(\epsilon )} \varphi_2, P_{\mathcal{H}, \mathcal{B}(\epsilon )} \varphi_2 \rangle_{\mathcal{A}(\epsilon )}\\
&= \langle e ^{-H(\epsilon )t} P_{\mathcal{H}, \mathcal{B}(\epsilon )} \varphi_2 -P_{\mathcal{H}, \mathcal{B}(\epsilon )} e^{-Ht} \varphi_2 ,P_{\mathcal{H}, \mathcal{B}(\epsilon )} \varphi_2\rangle _{\mathcal{A}(\epsilon )}\\
&\quad+e^{-\mu _2 t} \langle P_{\mathcal{H},\mathcal{B} (\epsilon )} \varphi_2, P_{\mathcal{H}, \mathcal{B}(\epsilon )} \varphi_2\rangle _{\mathcal{H}}\\
&= \langle e^{-H(\epsilon )t} P_{\mathcal{H}, \mathcal{B}(\epsilon )} \varphi_2 -P_{\mathcal{H}, \mathcal{B}(\epsilon )} e^{-Ht} \varphi_2, P_{\mathcal{H}, \mathcal{B}(\epsilon )} \varphi_2 \rangle _{\mathcal{A}(\epsilon )}\\
&\quad+ e^{-\mu_2 t} \langle (P_{\mathcal{H}, \mathcal{B}(\epsilon )} \varphi_2 -\varphi_2 )+\varphi_2,(P_{\mathcal{H}, \mathcal{B}(\epsilon )} \varphi_2 -\varphi_2 )+\varphi_2 \rangle _{\mathcal{H}}\\
&= \langle e^{-H(\epsilon )t} P_{\mathcal{H}, \mathcal{B}(\epsilon )} \varphi_2 -P_{\mathcal{H}, \mathcal{B}(\epsilon )} e^{-Ht} \varphi_2, P_{\mathcal{H}, \mathcal{B}(\epsilon )} \varphi_2 \rangle _{\mathcal{A}(\epsilon )}\\
&\quad+ e^{-\mu_2t} \{ \langle P_{\mathcal{H}, \mathcal{B}(\epsilon )} \varphi_2 -\varphi_2 ,P_{\mathcal{H}, \mathcal{B}(\epsilon )} \varphi_2 -\varphi_2\rangle_{\mathcal{H}}\\
&\quad+ 2\langle P_{\mathcal{H}, \mathcal{B}(\epsilon )} \varphi_2 -\varphi_2 ,\varphi_2\rangle _{\mathcal{H}} +1\}\\
&=  \langle e^{-H(\epsilon )t} P_{\mathcal{H},\mathcal{B}(\epsilon)} \varphi_2 -P_{\mathcal{H}, \mathcal{B}(\epsilon )} e^{-Ht}\varphi _2 ,P_{\mathcal{H}, \mathcal{B}(\epsilon )} \varphi_2 \rangle _{\mathcal{A}(\epsilon )}\\
&\quad+ e^{-\mu_2 t} \{ \langle P_{\mathcal{H}, \mathcal{B}(\epsilon )} \varphi_2 -\varphi_2 ,P_{\mathcal{H}, \mathcal{B}(\epsilon )} \varphi_2-\varphi_2\rangle_{\mathcal{H}}\\
&\quad+2 \langle P_{\mathcal{H}, \mathcal{B}(\epsilon )}
\varphi_2-\varphi_2, \varphi_2\rangle _{\mathcal{H}}\}
+ e^{-\mu_2 t}.
\end{align*}
Hence, by (A7) and (A28), we have
\begin{equation}\label{eq:2.21}
\lim_{\epsilon \downarrow 0}\langle e^{-H(\epsilon )t}
P_{\mathcal{H}, \mathcal{B}(\epsilon )} \varphi_2 ,
P_{\mathcal{H}, \mathcal{B}(\epsilon)} \varphi_2
\rangle _{\mathcal{A}(\epsilon )} = e^{-\mu_2 t}.
\end{equation}
Next we consider the term $\beta _1 (\epsilon)$ defined in
\eqref{eq:2.19}. We note that, by (A27),
\begin{equation}
\begin{split}\label{eq:2.22}
P_{\mathcal{A} (\epsilon ), \mathcal{B}(\epsilon )} \varphi_1 (\epsilon )&=\|P_{\mathcal{H}^{\epsilon _0}, \mathcal{A}(\epsilon )} \varphi_1^{\epsilon _0} \| ^{-1}_{\mathcal{A}(\epsilon)} P_{\mathcal{A}(\epsilon ), \mathcal{B}(\epsilon)} P_{\mathcal{H}^{\epsilon_0} , \mathcal{A}(\epsilon )} \varphi_1^{\epsilon _0}\\
&= \| P_{\mathcal{H}^{\epsilon_0}, \mathcal{A}(\epsilon )} \varphi^{\epsilon _0}_1\|^{-1}_{\mathcal{A}(\epsilon )} P_{\mathcal{H}^{\epsilon_0}, \mathcal{B}(\epsilon )} \varphi_1^{\epsilon _0}\\
&= \| P_{\mathcal{H}^{\epsilon _0}, \mathcal{A}(\epsilon)} \varphi_1^{\epsilon_0} \|^{-1}_{\mathcal{A}(\epsilon )} P_{\mathcal{H}, \mathcal{B}(\epsilon )} P_{\mathcal{H}^{\epsilon_0} , \mathcal{H}} \varphi_1^{\epsilon_0}\\
&=\| P_{\mathcal{H}^{\epsilon_0} , \mathcal{A}(\epsilon )}
\varphi_1^{\epsilon_0} \|^{-1}_{\mathcal{A}(\epsilon )}
\|P_{\mathcal{H}^{\epsilon_0}, \mathcal{H}}
 \varphi^{\epsilon _0}_1\|_{\mathcal{H}}P_{\mathcal{H},
\mathcal{B}(\epsilon )} \varphi_1.
\end{split}\end{equation}
Consider the term $\| P_{\mathcal{H}^{\epsilon_0},
\mathcal{A}(\epsilon)} \varphi^{\epsilon_0}_1
\|_{\mathcal{A}(\epsilon )}$ in \eqref{eq:2.22}.
We have, by (A9),
\begin{align*}
P_{\mathcal{H}^{\epsilon_0}, \mathcal{A}(\epsilon )}
\varphi^{\epsilon _0}_1 &=P_{\mathcal{H}^{\epsilon_0},
\mathcal{B}(\epsilon)} \varphi^{\epsilon_0}_1
+P_{\mathcal{H}^{\epsilon_0} , \mathcal{C}(\epsilon )}
\varphi^{\epsilon_0}_1 +P_{\mathcal{H}^{\epsilon_0},
\mathcal{D}(\epsilon)} \varphi^{\epsilon _0}_1\\
&=P_{\mathcal{H}, \mathcal{B}(\epsilon)} P_{\mathcal{H}^{\epsilon_0},
\mathcal{H}}\varphi^{\epsilon _0}_1+P_{\mathcal{H}^{\epsilon_0},
\mathcal{C}(\epsilon )} \varphi^{\epsilon _0}_1
 +P_{\mathcal{H}^{\epsilon_0}, \mathcal{D}(\epsilon )}
\varphi_1^{\epsilon_0}\\
&= \| P_{\mathcal{H}^{\epsilon_0}, \mathcal{H}}
\varphi^{\epsilon_0}_1 \|_{\mathcal{H}}
P_{\mathcal{H}, \mathcal{B}(\epsilon )} \varphi_1
+P_{\mathcal{H}^{\epsilon _0} , \mathcal{C}(\epsilon )}
\varphi_1^{\epsilon _0} +P_{\mathcal{H}^{\epsilon_0} ,
\mathcal{D}(\epsilon )} \varphi^{\epsilon_0}_1.
\end{align*}
Thus, by (A7), Lemma~\ref{lem:2.1} and (A10),
\begin{equation}
\begin{split}\label{eq:2.23}
\| P_{\mathcal{H}^{\epsilon _0} , \mathcal{A}(\epsilon )} \varphi_1^{\epsilon_0} \|^2_{\mathcal{A}(\epsilon )} &= \|P_{\mathcal{H}^{\epsilon _0} , \mathcal{H}} \varphi^{\epsilon _0}_1 \|^2_{\mathcal{H}} \| P_{\mathcal{H}, \mathcal{B}(\epsilon )} \varphi_1\| ^2_{\mathcal{B}(\epsilon )}\\
&\quad + \| P_{\mathcal{H}^{\epsilon _0} , \mathcal{C}(\epsilon )} \varphi^{\epsilon _0}_1 \|^2_{\mathcal{C}(\epsilon )} +\| P_{\mathcal{H}^{\epsilon _0}, \mathcal{D}(\epsilon )} \varphi^{\epsilon _0}_1\|^2_{\mathcal{D}(\epsilon )}\\
&=\| P_{\mathcal{H}^{\epsilon _0}, \mathcal{H}}  \varphi_1^{\epsilon _0} \|^2_{\mathcal{H}} \|(P_{\mathcal{H}, \mathcal{B}(\epsilon )} \varphi_1 -\varphi_1 )+\varphi_1 \|^2_{\mathcal{H}}\\
&\quad + \| P_{\mathcal{H}^{\epsilon _0}, \mathcal{C}(\epsilon )} \varphi^{\epsilon _0}_1\|^2_{\mathcal{C}(\epsilon )} +\|P_{\mathcal{H}^{\epsilon _0}, \mathcal{D}(\epsilon )}\varphi_1^{\epsilon _0} \|^2_{\mathcal{D}(\epsilon )}\\
&\to \| P_{\mathcal{H}^{\epsilon _0},\mathcal{H}}
 \varphi_1^{\epsilon _0} \|^2_{\mathcal{H}}\quad \text{as }
\epsilon \downarrow 0.
\end{split}\end{equation}
Thus, by (A9),
\begin{equation}
\begin{split}\label{eq:2.24}
\varphi_1 (\epsilon )&=P_{\mathcal{A}(\epsilon ),
\mathcal{B}(\epsilon )} \varphi_1 (\epsilon )
+P_{\mathcal{A}(\epsilon ), \mathcal{C} (\epsilon )}
 \varphi_1 (\epsilon )+P_{\mathcal{A}(\epsilon ),
\mathcal{D}(\epsilon )}\varphi_1 (\epsilon )\\
&=\| P_{\mathcal{H}^{\epsilon _0} , \mathcal{A}(\epsilon )}
 \varphi_1^{\epsilon _0} \|^{-1}_{\mathcal{A}(\epsilon )}
 \| P_{\mathcal{H}^{\epsilon _0} , \mathcal{H}}
\varphi^{\epsilon _0}_1\|_{\mathcal{H}} P_{\mathcal{H},
\mathcal{B}(\epsilon )} \varphi_1\\
&\quad + P_{\mathcal{A}(\epsilon ), \mathcal{C}(\epsilon )}
\varphi_1 (\epsilon )+P_{\mathcal{A}(\epsilon ),
\mathcal{D}(\epsilon )} \varphi_1 (\epsilon ).
\end{split}
\end{equation}
Since the second and third terms in the last line of \eqref{eq:2.24}
are in $\mathcal{C}(\epsilon )$ and $\mathcal{D}(\epsilon )$,
 respectively, they are orthogonal to
$P_{\mathcal{A}(\epsilon ),  \mathcal{B}(\epsilon )}
\varphi_1(\epsilon )$ by (A9). Hence, by \eqref{eq:2.24},
\eqref{eq:2.23} and (A7),
\begin{equation}\begin{split}\label{eq:2.25}
\beta _1 (\epsilon )
&=\langle P_{\mathcal{H}, \mathcal{B}(\epsilon )} \varphi_2 ,\varphi_1 (\epsilon )\rangle_{\mathcal{A}(\epsilon )}\\
&=\langle P_{\mathcal{H}, \mathcal{B} (\epsilon )}\varphi_2,\|P_{\mathcal{H}^{\epsilon _0}, \mathcal{A}(\epsilon )} \varphi^{\epsilon _0}_1 \|^{-1}_{\mathcal{A}(\epsilon )} \| P_{\mathcal{H}^{\epsilon _0}, \mathcal{H}} \varphi^{\epsilon _0}_1\|_{\mathcal{H}} P_{\mathcal{H}, \mathcal{B}(\epsilon )} \varphi_1\rangle _{\mathcal{H}}\\
&=\langle (P_{\mathcal{H}, \mathcal{B}(\epsilon )} \varphi_2 -\varphi_2)+\varphi_2, \| P_{\mathcal{H}^{\epsilon _0}, \mathcal{A}(\epsilon )} \varphi^{\epsilon _0}_1\|^{-1}_{\mathcal{A}(\epsilon )} \| P_{\mathcal{H}^{\epsilon _0}, \mathcal{H}}\varphi^{\epsilon _0}_1\|_{\mathcal{H}}\\
&\quad \times (P_{\mathcal{H}, \mathcal{B}(\epsilon )} \varphi_1 -\varphi_1)+\| P_{\mathcal{H}^{\epsilon _0}, \mathcal{A}(\epsilon )} \varphi_1^{\epsilon_0} \|^{-1}_{\mathcal{A}(\epsilon )} \| P_{\mathcal{H}^{\epsilon _0}, \mathcal{H}}\varphi^{\epsilon _0}_1\|_{\mathcal{H}} \varphi_1\rangle _{\mathcal{H}}\\
&\to \langle \varphi_2,\varphi_1\rangle _{\mathcal{H}}=0\quad
\text{as } \epsilon \downarrow 0.\end{split}\end{equation}
Therefore we can deal with the term
\[
 \| P_{\mathcal{H}, \mathcal{B}(\epsilon )} \varphi_2
-\beta_1 (\epsilon )\varphi_1 (\epsilon )\|^{-2}_{\mathcal{A}
(\epsilon )}
\] of \eqref{eq:2.20} as follows:
\begin{equation}\begin{split}\label{eq:2.26}
&\| P_{\mathcal{H}, \mathcal{B}(\epsilon )} \varphi_2 -\beta_1 (\epsilon )\varphi_1 (\epsilon )\|^{-2}_{\mathcal{A}(\epsilon )}\\
&= \| P_{\mathcal{H}, \mathcal{B}(\epsilon )}\varphi_2 -\beta_1 (\epsilon ) P_{\mathcal{A}(\epsilon ), \mathcal{B}(\epsilon )} \varphi_1 (\epsilon ) -\beta_1 (\epsilon )P_{\mathcal{A}(\epsilon ), \mathcal{C}(\epsilon )} \varphi_1 (\epsilon )\\
&\quad -\beta_1(\epsilon )P_{\mathcal{A}(\epsilon ), \mathcal{D}(\epsilon )} \varphi_1 (\epsilon )\|^{-2}_{\mathcal{A}(\epsilon )}\\
&=  \| P_{\mathcal{H}, \mathcal{B}(\epsilon )} \varphi_2 -\beta_1 (\epsilon )P_{\mathcal{A}(\epsilon ), \mathcal{B}(\epsilon )} \varphi_1 (\epsilon )\|^2_{\mathcal{B} (\epsilon )}\\
&\quad + \beta_1 (\epsilon )^2 \| P_{\mathcal{A}(\epsilon ), \, \mathcal{C}(\epsilon )} \varphi_1 (\epsilon ) \|^2_{\mathcal{C}(\epsilon )} +\beta_1(\epsilon )^2 \| P_{\mathcal{A}(\epsilon ), \, \mathcal{D}(\epsilon )} \varphi_1 (\epsilon )\|^2_{\mathcal{D} (\epsilon )}\\
&=  \|(P_{\mathcal{H}, \mathcal{B}(\epsilon )} \varphi_2 -\varphi_2 )+\varphi_2 -\beta _1 (\epsilon ) P_{\mathcal{A}(\epsilon ), \mathcal{B}(\epsilon )} \varphi_1 (\epsilon )\|^2_{\mathcal{H}}\\
&\quad +\beta _1 (\epsilon )^2\| P_{\mathcal{A}(\epsilon ), \mathcal{C}(\epsilon )} \varphi_1 (\epsilon )\|^2_{\mathcal{C}(\epsilon )} +\beta _1 (\epsilon )^2 \| P_{\mathcal{A}(\epsilon ), \mathcal{D}(\epsilon)} \varphi_1 (\epsilon )\|^2_{\mathcal{D}(\epsilon )}\\
&\to \| \varphi_2\|^2_{\mathcal{H}} =1\quad \text{as }
\epsilon \downarrow 0,
\end{split}\end{equation}
 by (A7) and \eqref{eq:2.25}.
Therefore, by \eqref{eq:2.20}, \eqref{eq:2.21}, \eqref{eq:2.25}
and \eqref{eq:2.26}, we have, for all $\delta >0$, there exists
$\epsilon _1\in (0,\epsilon _0]$ such that
\begin{equation}\label{eq:2.27}
\mu_2 (\epsilon )t\leq \mu_2 t+\delta
\end{equation}
for all $0<\epsilon \leq \epsilon _1$. We next prove the reverse
inequality of \eqref{eq:2.27}. For all $0<\epsilon \leq \epsilon_0$
let
\begin{equation}\label{eq:2.28}
\gamma _1 (\epsilon )=\langle P_{\mathcal{A}(\epsilon ),
\mathcal{B}(\epsilon )} \varphi_2 (\epsilon ),
\varphi_1\rangle_{\mathcal{H}}.
\end{equation}
Then
\begin{equation}\begin{split}\label{eq:2.29}
e^{-\mu_2 t}&\geq \|P_{\mathcal{A}(\epsilon ), \mathcal{B}(\epsilon )} \varphi_2 (\epsilon )-\gamma_1 (\epsilon )\varphi_1\|^{-2}_{\mathcal{H}}\\
&\quad \times \langle e^{-Ht} (P_{\mathcal{A}(\epsilon ),
 \mathcal{B}(\epsilon )} \varphi_2 (\epsilon ) -\gamma_1(\epsilon )\varphi_1), P_{\mathcal{A}(\epsilon ), \mathcal{B}(\epsilon )} \varphi_2 (\epsilon )-\gamma_1 (\epsilon )\varphi_1\rangle_{\mathcal{H}}\\
&=\| P_{\mathcal{A}(\epsilon ), \mathcal{B}(\epsilon )} \varphi_2 (\epsilon ) -\gamma_1 (\epsilon )\varphi_1 \|^{-2}_{\mathcal{H}}\\
&\quad \times \{ \langle e^{-Ht}P_{\mathcal{A}(\epsilon ), \mathcal{B}(\epsilon )} \varphi_2 (\epsilon ),P_{\mathcal{A}(\epsilon ), \mathcal{B}(\epsilon )} \varphi_2 (\epsilon )\rangle_{\mathcal{H}}\\
&\quad -2\gamma_1 (\epsilon )\langle e^{-Ht}P_{\mathcal{A}(\epsilon ), \mathcal{B} (\epsilon )} \varphi_2 (\epsilon ),\varphi_1\rangle_{\mathcal{H}} +\gamma_1 (\epsilon )^2\}\\
&=\| P_{\mathcal{A}(\epsilon ), \mathcal{B}(\epsilon )} \varphi_2(\epsilon )-\gamma_1 (\epsilon )\varphi_1\|^{-2}_{\mathcal{H}}\\
&\quad\times \{ \langle e^{-Ht}P_{\mathcal{A}(\epsilon ),
\mathcal{B}(\epsilon )} \varphi_2 (\epsilon ),P_{\mathcal{A}(\epsilon ), \mathcal{B}(\epsilon )}\varphi_2 (\epsilon )\rangle_{\mathcal{H}}-\gamma_1 (\epsilon )^2\}.\end{split}\end{equation}
Consider the term
\begin{equation}\begin{split}\label{eq:2.30}
 &\langle e^{-Ht} P_{\mathcal{A}(\epsilon ), \mathcal{B}(\epsilon )} \varphi_2 (\epsilon ),P_{\mathcal{A}(\epsilon ), \mathcal{B}(\epsilon )} \varphi_2(\epsilon )\rangle_{\mathcal{H}}\\
&= \langle e^{-Ht} P_{\mathcal{A}(\epsilon ), \mathcal{B}(\epsilon )} \varphi_2 (\epsilon )-P_{\mathcal{A}(\epsilon ), \mathcal{B}(\epsilon )} e^{-H(\epsilon )t} \varphi_2 (\epsilon ), P_{\mathcal{A}(\epsilon ), \mathcal{B}(\epsilon )} \varphi_2 (\epsilon )\rangle_{\mathcal{H}}\\
&\quad +\langle P_{\mathcal{A}(\epsilon ), \mathcal{B}(\epsilon )}e^{-H(\epsilon )t} \varphi_2 (\epsilon ),P_{\mathcal{A}(\epsilon ), \mathcal{B}(\epsilon )} \varphi_2(\epsilon )\rangle _{\mathcal{H}}\\
 &= \langle e^{-Ht}P_{\mathcal{A}(\epsilon ), \mathcal{B}(\epsilon )} \varphi_2 (\epsilon ) -P_{\mathcal{A}(\epsilon ), \mathcal{B}(\epsilon )} e^{-H(\epsilon )t} \varphi_2 (\epsilon ) ,P_{\mathcal{A}(\epsilon ), \mathcal{B}(\epsilon )} \varphi_2 (\epsilon )\rangle_{\mathcal{H}}\\
&\quad + e^{-\mu_2 (\epsilon )t} \langle P_{\mathcal{A}(\epsilon ),
\mathcal{B}(\epsilon )} \varphi_2 (\epsilon ),
P_{\mathcal{A}(\epsilon ), \mathcal{B}(\epsilon )} \varphi_2
(\epsilon )\rangle_{\mathcal{H}}.
\end{split}\end{equation}
Therefore, by (A28), \eqref{eq:2.27} and \eqref{eq:2.30},
for all $\delta >0$ there exists $\epsilon _1 \in (0,\epsilon _0]$
such that
\begin{equation}\label{eq:2.31}
\langle e^{-Ht} P_{\mathcal{A}(\epsilon ), \mathcal{B}(\epsilon )}
 \varphi_2 (\epsilon ) ,P_{\mathcal{A}(\epsilon ),
\mathcal{B}(\epsilon )} \varphi_2 (\epsilon )\rangle_{\mathcal{H}}
\geq e^{-\mu_2 (\epsilon )t-\delta }
\end{equation}
for all $\epsilon \in (0,\epsilon _1]$.

 We next consider the term $\gamma_1 (\epsilon )$ defined in
\eqref{eq:2.28}:
\begin{equation} \label{eq:2.32}
\gamma_1 (\epsilon )
=\langle P_{\mathcal{A}(\epsilon ), \mathcal{B}(\epsilon )}
  \varphi_2 (\epsilon ),\varphi_1\rangle _{\mathcal{H}}
=\langle P_{\mathcal{A}(\epsilon ), \mathcal{B}(\epsilon )}
  \varphi_2 (\epsilon ),P_{\mathcal{H}, \mathcal{B}(\epsilon )}
  \varphi_1 +P_{\mathcal{H}, \mathcal{B}(\epsilon ) ^\bot
  \mathcal{H}} \varphi_1 \rangle_{\mathcal{H}}.
\end{equation}
But, by (A27),
\begin{equation}\begin{split}\label{eq:2.33}
P_{\mathcal{H}, \mathcal{B}(\epsilon )} \varphi_1 &=\| P_{\mathcal{H}^{\epsilon _0}, \mathcal{H}}\varphi_1^{\epsilon _0} \|^{-1}_{\mathcal{H}} P_{\mathcal{H}, \mathcal{B}(\epsilon )} P_{\mathcal{H}^{\epsilon _0}, \mathcal{H}}\varphi^{\epsilon _0}_1\\
&=\| P_{\mathcal{H}^{\epsilon _0}, \mathcal{H}}\varphi_1^{\epsilon _0} \|^{-1}_{\mathcal{H}} P_{\mathcal{H}^{\epsilon _0}, \mathcal{B}(\epsilon)} \varphi^{\epsilon _0}_1\\
&=\| P_{\mathcal{H}^{\epsilon _0}, \mathcal{H}}\varphi^{\epsilon _0}_1 \|^{-1}_{\mathcal{H}} P_{\mathcal{A}(\epsilon ), \mathcal{B}(\epsilon )} P_{\mathcal{H}^{\epsilon _0}, \mathcal{A}(\epsilon )} \varphi^{\epsilon _0}_1\\
&= \| P_{\mathcal{H}^{\epsilon _0}, \mathcal{H}}
 \varphi^{\epsilon _0}_1\|^{-1}_{\mathcal{H}}\|
 P_{\mathcal{H}^{\epsilon_0}, \mathcal{A}(\epsilon )}
 \varphi^{\epsilon _0}_1 \| _{\mathcal{A}(\epsilon )}
 P_{\mathcal{A}(\epsilon ), \mathcal{B}(\epsilon )}
 \varphi_1 (\epsilon ).
\end{split}\end{equation}
Hence, from \eqref{eq:2.32} and \eqref{eq:2.33},
\begin{equation}\begin{split} \label{eq:2.34}
 \gamma_1(\epsilon )&=\langle P_{\mathcal{A}(\epsilon ), \mathcal{B}(\epsilon )} \varphi_2 (\epsilon ),\|P_{\mathcal{H}^{\epsilon _0}, \mathcal{H}}\varphi_1^{\epsilon_0}\|^{-1}_{\mathcal{H}} \| P_{\mathcal{H}^{\epsilon _0} , \mathcal{A}(\epsilon )}\varphi_1^{\epsilon_0} \|_{\mathcal{A}(\epsilon)}\\
&\quad \times P_{\mathcal{A}(\epsilon ), \mathcal{B}(\epsilon )} \varphi_1 (\epsilon) +P_{\mathcal{H}, \mathcal{B}(\epsilon)^\bot \mathcal{H}}\varphi_1\rangle _{\mathcal{H}}\\
&=\langle P_{\mathcal{A}(\epsilon ), \mathcal{B}(\epsilon)} \varphi_2 (\epsilon),\|P_{\mathcal{H}^{\epsilon_0}, \mathcal{H}}\varphi^{\epsilon_0}_1\|^{-1}_{\mathcal{H}}\| P_{\mathcal{H}^{\epsilon_0}, \mathcal{A}(\epsilon)}\varphi^{\epsilon_0}_1\|_{\mathcal{A}(\epsilon)}\\
&\quad \times P_{\mathcal{A}(\epsilon), \mathcal{B}(\epsilon)} \varphi_1(\epsilon)\rangle _{\mathcal{A}(\epsilon )} +\langle P_{\mathcal{A}(\epsilon ), \mathcal{B}(\epsilon )}\varphi_2 (\epsilon),P_{\mathcal{H}, \mathcal{B}(\epsilon)^\bot \mathcal{H}}\varphi_1\rangle_{\mathcal{H}}\\
&= \langle {P_{\mathcal{A}(\epsilon), \mathcal{B}(\epsilon)}}\varphi_2 (\epsilon) ,\| P_{\mathcal{H}^{\epsilon_0}, \mathcal{H}}\varphi^{\epsilon_0}_1\|^{-1}_{\mathcal{H}} \| P_{\mathcal{H}^{\epsilon_0}, \mathcal{A}(\epsilon)} \varphi^{\epsilon_0}_1\|_{\mathcal{A}(\epsilon)}\\
&\quad \times P_{\mathcal{A}(\epsilon), \mathcal{B}(\epsilon)}
 \varphi_1(\epsilon )\rangle _{\mathcal{A}(\epsilon)}.
\end{split}\end{equation}
We show that the last line of \eqref{eq:2.34} tends to $0$ as
$\epsilon\downarrow 0$:
We have
\begin{equation}\begin{split}\label{eq:2.35}
 0&= \langle \varphi_2(\epsilon),\varphi_1 (\epsilon)\rangle _{\mathcal{A}(\epsilon)}\\
&=\langle P_{\mathcal{A}(\epsilon), \mathcal{B}(\epsilon)} \varphi_2 (\epsilon),P_{\mathcal{A}(\epsilon), \mathcal{B}(\epsilon)} \varphi_1 (\epsilon)\rangle_{\mathcal{B}(\epsilon)}\\
&\quad + \langle P_{\mathcal{A}(\epsilon ), \mathcal{C}(\epsilon)}\varphi_2 (\epsilon),P_{\mathcal{A}(\epsilon), \mathcal{C}(\epsilon)} \varphi_1(\epsilon)\rangle _{\mathcal{C}(\epsilon)}\\
&\quad +\langle P_{\mathcal{A}(\epsilon ),
\mathcal{D}(\epsilon)} \varphi_2 (\epsilon),
P_{\mathcal{A}(\epsilon), \mathcal{D}(\epsilon)}
\varphi_1(\epsilon)\rangle_{\mathcal{D}(\epsilon)}.
\end{split}\end{equation}
Since, by (A28),
\begin{equation}\label{eq:2.36}
\lim_{\epsilon \downarrow 0}\|P_{\mathcal{A}(\epsilon ),
\mathcal{B}(\epsilon)} \varphi_n (\epsilon)\|_{\mathcal{B}
(\epsilon )}=1,\end{equation}
we have
\begin{equation}\label{eq:2.37}
\lim_{\epsilon \downarrow 0} \| P_{\mathcal{A}(\epsilon),
\mathcal{C}(\epsilon)} \varphi_n (\epsilon)\|_{\mathcal{C}(\epsilon)}
=\lim_{\epsilon\downarrow 0}\| P_{\mathcal{A}(\epsilon),
\mathcal{D}(\epsilon)} \varphi_n(\epsilon)\|_{\mathcal{D}(\epsilon)}=0.
\end{equation}
From \eqref{eq:2.35}, \eqref{eq:2.36} and \eqref{eq:2.37} we obtain
\begin{equation}\label{eq:2.38}
\lim_{\epsilon\downarrow 0} \langle P_{\mathcal{A}(\epsilon ),
\mathcal{B}(\epsilon)} \varphi_2 (\epsilon),P_{\mathcal{A}(\epsilon),
\mathcal{B}(\epsilon)}\varphi_1 (\epsilon)\rangle_{\mathcal{B}
(\epsilon)}=0.\end{equation}
 Hence, by \eqref{eq:2.34}, \eqref{eq:2.38} and \eqref{eq:2.23},
we have
\begin{equation}\label{eq:2.39}
\lim_{\epsilon \downarrow 0} \gamma_1 (\epsilon)=0.
\end{equation}
Thus, by \eqref{eq:2.39} and (A28), we have
\begin{equation}\begin{split}\label{eq:2.40}
&\| P_{\mathcal{A}(\epsilon ), \mathcal{B}(\epsilon )} \varphi_2 (\epsilon) -\gamma_1 (\epsilon )\varphi_1 \|^2_{\mathcal{H}}\\
&= \| P_{\mathcal{A}(\epsilon ), \mathcal{B}(\epsilon)} \varphi_2 (\epsilon)-\gamma_1 (\epsilon) P_{\mathcal{H}, \mathcal{B}(\epsilon)} \varphi_1
-\gamma_1 (\epsilon)P_{\mathcal{H}, \mathcal{B}(\epsilon)^\bot \mathcal{H}}\varphi_1 \|_{\mathcal{H}}^2\\
&= \| P_{\mathcal{A}(\epsilon ), \mathcal{B}(\epsilon)} \varphi_2 (\epsilon) -\gamma_1 (\epsilon )P_{\mathcal{H}, \mathcal{B}(\epsilon)} \varphi_1 \|^2_{\mathcal{B}(\epsilon)}
+\gamma_1 (\epsilon )^2 \|P_{\mathcal{H}, \mathcal{B}(\epsilon )^\bot \mathcal{H}}\varphi_1 \|^2_{\mathcal{H}}\\
& \to 1\quad \text{as } \epsilon\downarrow 0.
\end{split}\end{equation}
Combining \eqref{eq:2.29}, \eqref{eq:2.31}, \eqref{eq:2.39} and
\eqref{eq:2.40}, we see that for all $\delta >0$, there exists
$\epsilon _1 \in (0,\epsilon_0]$ such that
\begin{equation}\label{eq:2.41}
 \mu_2 t\leq \mu_2 (\epsilon )t+\delta
\end{equation}
for all $\epsilon \in (0,\epsilon_1]$. The theorem now follows
from \eqref{eq:2.27} and \eqref{eq:2.41}.
\end{proof}

\begin{definition}\label{def:2.21}\rm
 We now define the sequence $\{k_i\}^\infty_{i=1}$ of positive
integers as follows:
Suppose we list the eigenvalues $\{ \mu_n\}^\infty_{n=1}$ of $H$ in a way reflecting their multiplicities. Then the positive integers $k_i$ are defined by:
\begin{equation}\begin{split}\label{eq:2.42}
 0&=\mu_1 <\mu_2 =\mu_3 =\dots =\mu_{k_2}<\mu_{k_2+1}=\dots =\mu_{k_3}\\
&< \mu_{k_3+1}=\dots =\mu_{k_4}<\mu_{k_4+1}=\dots .
\end{split}\end{equation}
We also define $k_1=1$.
\end{definition}

\begin{lemma}\label{lem:2.22}
Let $p\geq 1$ be an integer and let $i$ be an integer satisfying
\[
k_p+1<i\leq k_{p+1}.
\]
Suppose, for $j=1,2,\dots$, $i-1$, we have
\begin{equation}\label{eq:2.43}
 \lim_{\epsilon \downarrow 0} \mu_j(\epsilon)=\mu_j.
\end{equation}
Then
\[
\lim_{\epsilon \downarrow 0} \mu_i (\epsilon)
=\mu_i=\mu_{k_p+1} =\mu_{k_{p+1}}.
\]
\end{lemma}

\begin{proof}
Assume, for a contradiction, that
\begin{equation}\label{eq:2.44}
\mu_i(\epsilon )\not\to\mu_i \quad \text{as }
\epsilon \downarrow 0.
\end{equation}
Then there exist $\eta >0$ and a strictly decreasing sequence
$\{\epsilon_m\}^\infty_{m=1}$ of positive numbers such that
$\epsilon_m\downarrow 0$ as $m\to \infty$,
and that
\[
\mu_i(\epsilon _m)\geq \mu_i+\eta \quad (m=1,2,3,\dots ).
\]
For $j=1,2,3,\dots $ we regard
$P_{\mathcal{H},\mathcal{B}(\epsilon)} \varphi_j$
as a vector in $\mathcal{A}(\epsilon )$ and write
\begin{equation}\label{eq:2.45}
P_{\mathcal{H}, \mathcal{B}(\epsilon)} \varphi_j
=\sum^\infty_{\ell=1} a_{j,\ell} (\epsilon )\varphi_{\ell} (\epsilon ).
\end{equation}
Then, for all $0<t\leq 1$ and $j=1,2,3,\dots $,
\begin{equation}\begin{split}\label{eq:2.46}
& e^{-H(\epsilon )t} P_{\mathcal{H}, \mathcal{B}(\epsilon )} \varphi_j -P_{\mathcal{H}, \mathcal{B}(\epsilon )} e^{-Ht}\varphi_j\\
&= \Big(\sum^{i-1}_{\ell =1} +\sum^\infty_{\ell=i}\Big) a_{j,\ell}
(\epsilon )(e^{-\mu_\ell (\epsilon )t} -e ^{-\mu_jt}) \varphi_\ell
(\epsilon).\end{split}\end{equation}
By (A28), \eqref{eq:2.43}, \eqref{eq:2.46} and the orthogonality
of $\{ \varphi _i(\epsilon )\}^\infty_{i=1}$, we have
\begin{equation}\label{eq:2.47}
\lim_{\epsilon\downarrow 0} \sum^\infty_{\ell=i} a_{j,\ell}
(\epsilon)^2 (e^{-\mu_\ell (\epsilon )t}-e ^{-\mu_jt})^2=0.
\end{equation}
Since, for $\ell =i,i+1,i+2,\dots $ and $j=1,2,\dots$, $k_{p+1}$
and $m=1,2,3,\dots$, we have
$\mu_{\ell}(\epsilon_m)\geq \mu_j+\eta$.
Equation \eqref{eq:2.47} implies
\[
\lim_{m\to \infty}\sum^\infty_{\ell=i} a_{j,\ell} (\epsilon_m)^2=0.
\]
Hence, for $j=1,2,\dots $, $k_{p+1}$,
\begin{equation}\label{eq:2.48}
\lim_{m\to \infty} \big\|\sum^\infty_{\ell=i}a_{j,\ell }
(\epsilon_m)\varphi_\ell (\epsilon_m)\big\|_{\mathcal{A}(\epsilon_m)}
=0.\end{equation}
Since, by (A7),
$\lim_{\epsilon \downarrow 0}\|P_{\mathcal{H},
\mathcal{B}(\epsilon)} \varphi_j\|_{\mathcal{A}(\epsilon)}=1$,
 \eqref{eq:2.48} implies that, for $j=1,2,\dots$, $k_{p+1}$,
\begin{equation}\label{eq:2.49}
\lim_{m\to \infty} \big\| \sum^{i-1}_{\ell=1} a_{j,\ell}
(\epsilon_m)\varphi_\ell (\epsilon_m)\big\| _{\mathcal{A}
(\epsilon _m)}=1.
\end{equation}
For $j=1,2,\dots $, $k_{p+1}$ and $m=1,2,3,\dots $ let
\begin{equation}\label{eq:2.50}
 u_{j,i}(m)=\sum^{i-1}_{\ell=1} a_{j,\ell}(\epsilon _m)
\varphi_\ell (\epsilon _m).
\end{equation}
Then, for $\sigma ,\tau \in \{ 1,2,\dots ,i\}$ with
$\sigma \neq \tau$, we have
\begin{equation}\begin{split}\label{eq:2.51}
 &\langle P_{\mathcal{H}, \mathcal{B}(\epsilon)} \varphi_\sigma ,P_{\mathcal{H}, \mathcal{B}(\epsilon)}\varphi_\tau \rangle _{\mathcal{B}(\epsilon)}\\
&= \langle \varphi_\sigma ,\varphi_\tau \rangle _{\mathcal{H}}-\langle (I_{\mathcal{H}}-P_{\mathcal{H}, \mathcal{B}(\epsilon)} )\varphi_\sigma ,(I_{\mathcal{H}}-P_{\mathcal{H}, \mathcal{B}(\epsilon)} )\varphi_\tau \rangle_{\mathcal{B}(\epsilon )^\bot \mathcal{H}}\\
&\to 0 \quad \text{as } \epsilon \downarrow 0 \text{ (by (A7))}.
\end{split}\end{equation}
But for $m=1,2,3,\dots $
\begin{equation}\begin{split}\label{eq:2.52}
&\langle P_{\mathcal{H}, \mathcal{B}(\epsilon _m)}\varphi_\sigma ,P_{\mathcal{H}, \mathcal{B}(\epsilon_m)}\varphi_\tau\rangle _{\mathcal{B}(\epsilon_m)}\\
&=  \langle u_{\sigma ,i}(m),u_{\tau ,i}(m)\rangle _{\mathcal{A}(\epsilon_m)}\\
&\quad +\big\langle \sum^\infty_{\ell=i}a_{\sigma ,\ell}
(\epsilon_m)\varphi_{\ell }(\epsilon_m),\sum^\infty_{\ell=i}
a_{\tau ,\ell}(\epsilon_m)\varphi_\ell (\epsilon_m)
\big\rangle_{\mathcal{A}(\epsilon_m)}.
\end{split}\end{equation}
From \eqref{eq:2.48}, \eqref{eq:2.51} and \eqref{eq:2.52}, we obtain
\begin{equation} \label{eq:2.53}
\lim_{m\to \infty} \langle u_{\sigma ,i}(m),u_{\tau ,i}(m)
\rangle_{\mathcal{A}(\epsilon _m)}=0.
\end{equation}
From \eqref{eq:2.49}, \eqref{eq:2.50} and \eqref{eq:2.53},
we have a set of $i$ vectors $\{u_{1,i}(m),\dots ,u_{i,i}(m)\}$ in
an $(i-1)$-dimensional inner product space spanned by
$\{ \varphi_1(\epsilon _m),\dots ,\varphi_{i-1}(\epsilon_m)\}$ which,
as $m\to \infty$, is almost orthonormal. This gives a contradiction.
Thus we must have
$\lim_{\epsilon \downarrow 0} \mu_i (\epsilon)
=\mu_i$.
\end{proof}

\begin{lemma}\label{lem:2.23}
Let $p\geq 2$ be an integer. Suppose that
$\lim_{\epsilon\downarrow 0} \mu_i(\epsilon )=\mu_i$
for all $i=1,2,\dots, k_p$. Then there exists $\eta >0$ such that
for all sufficiently small $\epsilon>0$ we have
\[
\mu_{k_p+1} (\epsilon)\geq \mu_{k_p}+\eta.
\]
\end{lemma}

\begin{proof}
 For $i=1,2,3,\dots$ let
\begin{equation}\label{eq:2.54} P_{\mathcal{A}(\epsilon ),
 \mathcal{B}(\epsilon)} \varphi_i (\epsilon)
=\sum^\infty_{\ell=1} b_{i,\ell} (\epsilon)\varphi_\ell ,
\end{equation}
regarding $P_{\mathcal{A}(\epsilon),\mathcal{B}(\epsilon)}
\varphi_i(\epsilon)$ as a vector in $\mathcal{H}$. Suppose the
lemma is false. Then there exists a strictly decreasing sequence
of positive numbers $\{ \epsilon_m\}^\infty_{m=1}$ such that
$\epsilon_m\downarrow 0$ as $m\to \infty$
 and that
\begin{equation}\label{eq:2.55}
 \mu_{k_p+1}(\epsilon _m)\to \mu_{k_p} \quad \text{as }
m\to \infty.
\end{equation}
Then, for all $0<t\leq 1$ and $n=1,2,3,\dots$, we have
\begin{equation}\begin{split}\label{eq:2.56}
& e^{-Ht} P_{\mathcal{A}(\epsilon ), \mathcal{B}(\epsilon )}
 \varphi_n (\epsilon) -P_{\mathcal{A}(\epsilon),
 \mathcal{B}(\epsilon)} e^{-H(\epsilon)t} \varphi_n(\epsilon)\\
&= \Big(\sum^{k_{p-1}}_{\ell =1} +\sum^{k_p}_{\ell=k_{p-1}+1}
+\sum^\infty_{\ell=k_p+1}\Big) b_{n,\ell }(\epsilon )
(e^{-\mu_\ell t}-e^{-\mu_n(\epsilon )t})\varphi_\ell\\
&=  A+B+C.\end{split}\end{equation}
By (A28) and the orthogonality of $\{ \varphi_\ell\}^\infty_{\ell=1}$
we have
\begin{equation}\label{eq:2.57}
 \lim_{\epsilon \downarrow 0} \| A\|_{\mathcal{H}}
=\lim_{\epsilon \downarrow 0} \| B\|_{\mathcal{H}}
=\lim_{\epsilon \downarrow 0}\| C\|_{\mathcal{H}}=0.
\end{equation}
For $n=k_{p-1}+1,\dots , k_p+1$, \eqref{eq:2.55} and \eqref{eq:2.57}
imply
\begin{equation}\label{eq:2.58}
\lim_{m\to \infty}\Big\{ \sum^{k_{p-1}}_{\ell=1} b_{n,\ell}
(\epsilon_m)^2 +\sum^\infty_{\ell=k_p+1} b_{n,\ell }
(\epsilon_m)^2\Big\} =0.
\end{equation}
Using (A28) and \eqref{eq:2.58} we obtain
\begin{equation}\label{eq:2.59}
\lim_{m\to \infty} \big\| \sum^{k_p}_{\ell=k_{p-1}+1}
b_{n,\ell} (\epsilon_m)\varphi_\ell \big\|_{\mathcal{H}}=1
\end{equation}
for all $n=k_{p-1}+1,\dots ,k_p+1$.

For $\sigma ,\tau \in \{ k_{p-1}+1,\dots ,k_p+1\}$ with
$\sigma \neq \tau$, we have
\begin{equation}\begin{split}0
&= \langle \varphi_\sigma (\epsilon ),\varphi_\tau (\epsilon)
 \rangle _{\mathcal{A}(\epsilon )}\\
&= \langle P_{\mathcal{A}(\epsilon), \mathcal{B}(\epsilon)}
 \varphi_\sigma (\epsilon),P_{\mathcal{A}(\epsilon ),
 \mathcal{B}(\epsilon)} \varphi_\tau (\epsilon )
 \rangle _{\mathcal{B}(\epsilon)}\\
&\quad + \langle P_{\mathcal{A}(\epsilon ),\mathcal{C}(\epsilon )
 \oplus \mathcal{D}(\epsilon )} \varphi_\sigma(\epsilon),
 P_{\mathcal{A}(\epsilon ),\mathcal{C}(\epsilon )\oplus
 \mathcal{D}(\epsilon)}\varphi_\tau (\epsilon )
 \rangle_{\mathcal{C}(\epsilon )\oplus \mathcal{D}(\epsilon )}
\end{split}\end{equation}
and since
\begin{equation}\label{eq:2.61} 1
=\| \varphi_\sigma (\epsilon )\|^2_{\mathcal{A}(\epsilon )}
=\| P_{\mathcal{A}(\epsilon ), \mathcal{B}(\epsilon )}\varphi_\sigma (\epsilon )\|^2_{\mathcal{B}(\epsilon)}
+ \| P_{\mathcal{A}(\epsilon ) ,\mathcal{C}(\epsilon )\oplus
\mathcal{D}(\epsilon )} \varphi_\sigma (\epsilon
)\|^2_{\mathcal{C}(\epsilon )\oplus \mathcal{D}(\epsilon
)}\end{equation}
 and
\begin{equation}\label{eq:2.62}
\lim_{\epsilon \downarrow 0} \| P_{\mathcal{A}(\epsilon ),
\mathcal{B}(\epsilon )}\varphi_\sigma (\epsilon )\|^2_{\mathcal{B}
(\epsilon)}=1,
\end{equation}
 we have
\begin{equation}\label{eq:2.63}
\lim_{\epsilon \downarrow 0} \langle P_{\mathcal{A}(\epsilon ),
\mathcal{B}(\epsilon)}\varphi_\sigma
(\epsilon),P_{\mathcal{A}(\epsilon ), \mathcal{B}(\epsilon )}
\varphi_\tau (\epsilon )\rangle_{\mathcal{B}(\epsilon )}=0.
\end{equation}
 Hence, from \eqref{eq:2.54}, \eqref{eq:2.58}, \eqref{eq:2.59}
and \eqref{eq:2.63}, we have
\begin{equation}\label{eq:2.64}
\lim_{m\to \infty} \Big\langle \sum^{k_p}_{\ell =k_{p-1} +1}
 b_{\sigma ,\ell} (\epsilon _m)\varphi_\ell ,
\sum^{k_p}_{\ell=k_{p-1}+1} b_{\tau ,\ell} (\epsilon _m)\varphi_\ell
\Big\rangle_{\mathcal{H}}=0.
\end{equation}
For $n=k_{p-1} +1,\dots $, $k_p+1$ and $m=1,2,3,\dots $ let
\begin{equation}\label{eq:2.65}
u_n(m)=\sum^{k_p}_{\ell=k_{p-1}+1} b_{n,\ell }(\epsilon _m)
\varphi_\ell .
\end{equation}
Then we have a set of $k_p+1-k_{p-1}$ vectors
$\{ u_{k_{p-1}+1}(m),\dots , u_{k_p+1}(m)\}$ in a
$(k_p-k_{p-1})$-dimensional inner product space spanned by the
set $\{ \varphi_{k_{p-1}+1},\dots ,\varphi_{k_p}\}$ which,
 by \eqref{eq:2.59} and \eqref{eq:2.64}, is almost orthonormal.
This gives a contradiction. Hence \eqref{eq:2.55} cannot be true
and the lemma is proved.
\end{proof}

\begin{lemma}\label{lem:2.24}
Let $p\geq 2$ be an integer. Suppose that
$\lim_{\epsilon \downarrow 0}\mu_i(\epsilon )=\mu_i$
for $i=1,2,\dots ,k_p$. Then
\[
\lim_{\epsilon \downarrow 0} \mu_{k_p+1}(\epsilon )=\mu_{k_p+1}.
\]
\end{lemma}

\begin{proof}
For $0<\epsilon \leq \epsilon _0$ let
\begin{equation}\label{eq:2.66}
P_{\mathcal{H}, \mathcal{B}(\epsilon)} \varphi_{k_p+1}
=\sum^\infty_{\ell =1} \beta_\ell (\epsilon )\varphi_\ell
(\epsilon)\end{equation}
regarded as a vector in $\mathcal{A}(\epsilon)$ and let
\begin{equation}\label{eq:2.67}
f_{k_p+1} (\epsilon )=P_{\mathcal{H}, \mathcal{B}(\epsilon)}
\varphi_{k_p+1}-\sum^{k_p}_{\ell =1} \beta_\ell (\epsilon)
\varphi_\ell (\epsilon)\in \mathcal{A}(\epsilon ).
\end{equation}
Then
\begin{align} %\label{eq:2.68}
&e ^{-\mu_{k_p+1}(\epsilon )t} \nonumber\\
&\geq \| f_{k_p+1} (\epsilon )\|
^{-2}_{\mathcal{A}(\epsilon )} \langle e^{-H(\epsilon )t}
f_{k_p+1}(\epsilon ),f_{k_p+1}(\epsilon )\rangle_{\mathcal{A}
(\epsilon)} \nonumber\\
&=\|f_{k_p+1}(\epsilon )\|^{-2}_{\mathcal{A}(\epsilon)}
\Big\langle e^{-H(\epsilon )t} P_{\mathcal{H},
 \mathcal{B}(\epsilon)}\varphi_{k_p+1} -\sum^{k_p}_{\ell =1}
\beta_\ell (\epsilon )e^{-\mu_\ell (\epsilon )t}\varphi_\ell
(\epsilon ),\nonumber\\
&\quad P_{\mathcal{H}, \mathcal{B}(\epsilon)} \varphi_{k_p+1}
-\sum^{k_p}_{\ell =1} \beta _\ell (\epsilon ) \varphi_
\ell (\epsilon )\Big\rangle _{\mathcal{A}(\epsilon)} \nonumber\\
&=\| f_{k_p+1}(\epsilon )\|^{-2}_{\mathcal{A}(\epsilon)}
\Big\{ \langle e^{-H(\epsilon )t} P_{\mathcal{H},
\mathcal{B}(\epsilon)} \varphi_{k_p+1},P_{\mathcal{H},
\mathcal{B}(\epsilon)}\varphi_{k_p+1}\rangle_{\mathcal{A}
(\epsilon)} \nonumber\\
&\quad -2\Big\langle\sum^{k_p}_{\ell =1} \beta_\ell (\epsilon)
 e^{-\mu_\ell (\epsilon )t} \varphi_\ell (\epsilon),
P_{\mathcal{H}, \mathcal{B}(\epsilon )} \varphi_{k_p+1}
\Big\rangle_{\mathcal{A}(\epsilon )}
 +\sum^{k_p}_{\ell=1} e^{-\mu_\ell (\epsilon )t}
\beta_\ell (\epsilon )^2\Big\}  \nonumber \\
&=\| f_{k_p+1} (\epsilon )\|^{-2}_{\mathcal{A}(\epsilon )}
\Big\{ \langle e^{-H(\epsilon )t} P_{\mathcal{H},
\mathcal{B}(\epsilon )}\varphi_{k_p+1} -P_{\mathcal{H},
 \mathcal{B}(\epsilon )} e^{-Ht} \varphi_{k_p+1}, \nonumber\\
&\quad P_{\mathcal{H},
\mathcal{B}(\epsilon)}\varphi_{k_p+1}\rangle_{\mathcal{A}(\epsilon)}
+ \langle  P_{\mathcal{H}, \mathcal{B}(\epsilon)}e^{-Ht}
\varphi_{k_p+1},P_{\mathcal{H},
\mathcal{B}(\epsilon)}\varphi_{k_p+1}\rangle_{\mathcal{A}(\epsilon)}
 \nonumber\\
&\quad -  \sum^{k_p}_{\ell =1} e ^{-\mu_\ell (\epsilon )t}
  \beta_\ell (\epsilon)^2\Big\}  \label{eq:2.68}\\
&= \| f_{k_p+1} (\epsilon )\|^{-2}_{\mathcal{A}(\epsilon )}
\Big\{ \langle e^{-H(\epsilon )t} P_{\mathcal{H},
\mathcal{B}(\epsilon )} \varphi_{k_p+1} -P_{\mathcal{H},
\mathcal{B}(\epsilon )} e^{-Ht} \varphi_{k_p+1}, \nonumber\\
&\quad P_{\mathcal{H}, \mathcal{B}(\epsilon )} \varphi_{k_p+1}
\rangle_{\mathcal{A}(\epsilon )} + e^{-\mu_{k_p+1}t}
\sum^\infty_{\ell =1} \beta_\ell (\epsilon )^2 \nonumber\\
&\quad -  \sum^{k_p}_{\ell =1} e^{-\mu_\ell (\epsilon )t}\beta_\ell
(\epsilon )^2\Big\}. \nonumber
\end{align}
Now
\begin{equation}\begin{split}\label{eq:2.69}
&e^{-H(\epsilon )t} P_{\mathcal{H}, \mathcal{B}(\epsilon )}
 \varphi_{k_p+1}-P_{\mathcal{H}, \mathcal{B}(\epsilon )}
 e^{-Ht}\varphi_{k_p+1}\\
&=  \sum^\infty_{\ell=1} \beta_\ell (\epsilon )
 (e^{-\mu_\ell (\epsilon )t} -e ^{-\mu _{k_p+1}t} )
 \varphi_\ell (\epsilon ).
\end{split}\end{equation}
So, by (A28), we have
\begin{equation}\label{eq:2.70}
\lim_{\epsilon \downarrow 0} \sum^\infty_{\ell =1}
\beta_\ell (\epsilon )^2 (e^{-\mu_\ell (\epsilon )t}
-e^{-\mu _{k_p+1}t} )^2=0,
\end{equation}
in particular
\begin{equation}\label{eq:2.71}
\lim_{\epsilon \downarrow 0}\sum^{k_p}_{\ell =1}
\beta_\ell (\epsilon )^2 (e^{-\mu_\ell (\epsilon ) t}
-e^{-\mu _{k_p+1}t} )^2=0.
\end{equation}
But for $\ell=1,\dots,k_p$ we have, by assumption,
$\lim_{\epsilon \downarrow 0} \mu_\ell (\epsilon )=\mu_\ell$.
Hence \eqref{eq:2.71} implies
\begin{equation}\label{eq:2.72}
\lim_{\epsilon \downarrow 0} \sum^{k_p}_{\ell=1}
\beta_\ell (\epsilon )^2=0.
\end{equation}
So, by (A7), \eqref{eq:2.67} and \eqref{eq:2.72}, we have
\begin{equation}\label{eq:2.73}
\lim_{\epsilon \downarrow 0} \sum^\infty_{\ell=k_p+1}
\beta_\ell (\epsilon )^2=\lim_{\epsilon \downarrow 0}
\| f_{k_p+1} (\epsilon )\|^2_{\mathcal{A}(\epsilon )}=1.
\end{equation}
From \eqref{eq:2.68}, \eqref{eq:2.69}, \eqref{eq:2.70}, \eqref{eq:2.72}, (A7) and \eqref{eq:2.66}, we have for all $\delta >0$ there exists $\epsilon _1\in (0,\epsilon _0]$ such that
\begin{equation}\label{eq:2.74}
e^{-\mu_{k_p+1}(\epsilon) t}\geq e^{-\mu_{k_p+1}t}-\delta
\end{equation}
for all $\epsilon \in (0,\epsilon_1]$.

 Next we prove the reverse inequality of \eqref{eq:2.74}.
For $i=1,2,3,\dots$ and $\epsilon \in (0,\epsilon_0]$, let
\begin{equation}\label{eq:2.75}
P_{\mathcal{A}(\epsilon ), \mathcal{B}(\epsilon )}
\varphi_i(\epsilon )=\sum^\infty_{\ell=1} \gamma_{i,\ell}
(\epsilon )\varphi_\ell \in \mathcal{B}(\epsilon )\subseteq
\mathcal{H}
\end{equation}
and let
\begin{equation}\label{eq:2.76}
g_{k_p+1} (\epsilon )=P_{\mathcal{A}(\epsilon ),
\mathcal{B}(\epsilon)} \varphi_{k_p+1} (\epsilon )
-\sum^{k_p}_{\ell=1} \gamma _{k_p+1,\ell}(\epsilon )\varphi_\ell .
\end{equation}
Then
%\label{eq:2.77}
\begin{align}
&e^{-\mu_{k_p+1}t} \nonumber\\
&\geq \| g_{k_p+1} (\epsilon )\| _{\mathcal{H}}^{-2}
 \langle e^{-Ht}g_{k_p+1}(\epsilon ),g_{k_p+1} (\epsilon )
 \rangle _{\mathcal{H}} \nonumber\\
&=\| g_{k_p+1} (\epsilon )\|^{-2}_{\mathcal{H}}\{\langle
 e^{-Ht} P_{\mathcal{A}(\epsilon ),
 \mathcal{B}(\epsilon)}\varphi_{k_p+1} (\epsilon ),
 P_{\mathcal{A}(\epsilon ), \mathcal{B}(\epsilon)}
 \varphi_{k_p+1}(\epsilon )\rangle_{\mathcal{H}} \nonumber\\
&\quad -2\Big\langle e^{-Ht}P_{\mathcal{A}(\epsilon ),
\mathcal{B}(\epsilon) } \varphi_{k_p+1} (\epsilon ),
 \sum^{k_p}_{\ell =1} \gamma _{k_p+1,\ell} (\epsilon )\varphi_\ell
\Big\rangle _{\mathcal{H}} \nonumber\\
&\quad + \Big\langle e^{-Ht} \sum^{k_p}_{\ell =1}
\gamma_{k_{p+1, \ell}} (\epsilon )\varphi_\ell ,
\sum^{k_p}_{\ell=1}\gamma_{k_p+1,\ell}(\epsilon )\varphi_\ell
\Big\rangle_{\mathcal{H}}\Big\} \nonumber\\
&=\| g_{k_p+1} (\epsilon ) \|^{-2}_{\mathcal{H}}
 \Big\{ \langle e^{-Ht} P_{\mathcal{A}(\epsilon ),
 \mathcal{B}(\epsilon )} \varphi_{k_p+1}(\epsilon )
 -P_{\mathcal{A}(\epsilon ), \mathcal{B}(\epsilon )}
 e^{-H(\epsilon )t} \varphi_{k_p+1} (\epsilon ), \nonumber\\
& \quad  P_{\mathcal{A}(\epsilon ), \mathcal{B}(\epsilon )}
 \varphi_{k_p+1} (\epsilon )\rangle _{\mathcal{H}}
 +\langle P_{\mathcal{A}(\epsilon ), \mathcal{B}(\epsilon )}
 e^{-H(\epsilon )t} \varphi_{k_p+1} (\epsilon ), \nonumber\\
& \quad  P_{\mathcal{A}(\epsilon ), \mathcal{B}(\epsilon )}
  \varphi_{k_p+1} (\epsilon )\rangle _{\mathcal{H}}
 -2\sum^{k_p}_{\ell =1} e^{-\mu _\ell t} \gamma_{k_p+1, \ell}
 (\epsilon )^2 \nonumber \\
&\quad +\sum_{\ell=1}^{k_p} e^{-\mu _\ell t}
\gamma_{k_p+1,\ell } (\epsilon )^2\Big\} \label{eq:2.77} \\
&= \| g_{k_p+1} (\epsilon )\|^{-2}_{\mathcal{H}}
 \Big\{ \langle e^{-Ht}
 P_{\mathcal{A}(\epsilon ), \mathcal{B}(\epsilon )} \varphi_{k_p+1}
 (\epsilon ) -P_{\mathcal{A}(\epsilon ), \mathcal{B}(\epsilon )}
 e^{-H(\epsilon )t} \varphi_{k_p+1} (\epsilon ), \nonumber\\
& \quad  P_{\mathcal{A}(\epsilon ), \mathcal{B}(\epsilon )}
 \varphi_{k_p+1} (\epsilon )\rangle_{\mathcal{H}}
 + e^{-\mu_{k_p+1}(\epsilon )t} \sum^\infty_{\ell=1}
 \gamma_{k_p+1,\ell}(\epsilon )^2 \nonumber\\
& \quad  - \sum^{k_p}_{\ell =1} e^{-\mu _\ell t}
\gamma _{k_p+1,\ell } (\epsilon )^2\Big\}. \nonumber
\end{align}
Now, by (A28),
\begin{equation}\begin{split}\label{eq:2.78}
&\| e^{-Ht} P_{\mathcal{A}(\epsilon ), \mathcal{B}(\epsilon )}
 \varphi_{k_p+1}(\epsilon ) -P_{\mathcal{A}(\epsilon ),
 \mathcal{B}(\epsilon )} e^{-H(\epsilon )t} \varphi_{k_p+1}
 (\epsilon )\|^2_{\mathcal{H}}\\
&= \sum^{\infty}_{\ell =1} \gamma_{k_p+1,\ell }(\epsilon )^2
 (e ^{-\mu_\ell t} - e ^{-\mu _{k_p+1} (\epsilon )t} )^2
 \to  0 \quad \text{as } \epsilon \downarrow 0,
\end{split}\end{equation}
in particular we have
\begin{equation}\label{eq:2.79}
\lim_{\epsilon \downarrow 0} \sum^{k_p}_{\ell =1}
\gamma _{k_p+1,\ell} (\epsilon )^2 (e^{-\mu_\ell t}
- e^{-\mu_{k_p+1}(\epsilon )t} )^2=0.
\end{equation}
But, by Lemma~\ref{lem:2.23}, there exists $\eta >0$ such that
for all sufficiently small $\epsilon >0$ we have
\begin{equation}\label{eq:2.80}
\mu_{k_p+1} (\epsilon )\geq \mu_{k_p}+\eta .
\end{equation}
Thus, from \eqref{eq:2.79} and \eqref{eq:2.80}, we have
\begin{equation}\label{eq:2.81}
 \lim_{\epsilon \downarrow 0} \sum^{k_p}_{\ell =1} \gamma_{k_p+1,\ell } (\epsilon)^2=0.\end{equation}
Hence, by (A28), \eqref{eq:2.81} and \eqref{eq:2.76}, we obtain
\begin{equation}\label{eq:2.82}
 \lim_{\epsilon \downarrow 0} \| g_{k_p+1}
(\epsilon )\|_{\mathcal{H}}=1.\end{equation}
Therefore, by \eqref{eq:2.75}, \eqref{eq:2.77}, \eqref{eq:2.81},
\eqref{eq:2.82} and (A28), given any $\delta >0$, there exists
$\epsilon_1 \in (0,\epsilon _0]$ such that
\begin{equation}\label{eq:2.83}
 e^{-\mu_{k_p+1}t}\geq e^{-\mu_{k_p+1}(\epsilon )t}-\delta
\end{equation}
for all $\epsilon \in (0,\epsilon_1]$. The lemma now follows
from \eqref{eq:2.74} and \eqref{eq:2.83}.
\end{proof}

\begin{theorem}\label{thm:2.25}
 For all $i=1,2,3,\dots$, we have
$ \lim_{\epsilon \downarrow 0} \mu_i(\epsilon )=\mu_i$.
\end{theorem}

The above theorem follows from Theorem~\ref{thm:2.20},
and  Lemmas~\ref{lem:2.22}
and \ref{lem:2.24}.

\begin{theorem}\label{thm:2.26}
For all $j=1,2,3,\dots $ and $\epsilon \in (0,\epsilon _0]$ let
\begin{equation}\label{eq:2.84}
P_{\mathcal{H}, \mathcal{B}(\epsilon)}\varphi_j
=\sum^\infty_{\ell =1} a_{j,\ell} (\epsilon )\varphi_\ell (\epsilon )
\in \mathcal{B}(\epsilon )\subseteq \mathcal{A}(\epsilon ).
\end{equation}
Let $p\geq 1$ be an integer. For $i=k_p+1,\dots$, $k_{p+1}$ and
$\epsilon \in (0,\epsilon_0]$ let
\begin{equation}\label{eq:2.85}
\hat{\psi}_i (\epsilon )=P_{\mathcal{A}(\epsilon ),
\mathcal{B}(\epsilon )}\Big(\sum^{k_{p+1}}_{\ell =k_p+1} a_{i,\ell}
(\epsilon )\varphi_\ell (\epsilon )\Big)
\end{equation}
and let
\begin{equation}\label{eq:2.86}
\psi_{i}(\epsilon )=\|\hat{\psi}_i(\epsilon )
\|^{-1}_{\mathcal{B}(\epsilon )} \hat{\psi}_i (\epsilon ).
\end{equation}
Then for each $i=k_p+1,\dots ,k_{p+1}$ we have
\begin{equation}\label{eq:2.87}
\lim_{\epsilon \downarrow 0} \| \varphi_i
-\psi _i (\epsilon )\|_{\mathcal{H}} =0.
\end{equation}
\end{theorem}

\begin{proof}
For $i=k_p+1,\dots ,k_{p+1}$ and $\epsilon \in (0,\epsilon_0]$ we have
\begin{equation}\begin{split}\label{eq:2.88}
&\| \varphi_i-\psi_i(\epsilon )\|_{\mathcal{H}}\\
&\leq \| \varphi_i-P_{\mathcal{H}, \mathcal{B}(\epsilon )}
 \varphi_i \| _{\mathcal{H}}+ \| P_{\mathcal{H},
 \mathcal{B}(\epsilon )} \varphi_i -\hat{\psi }_i
 (\epsilon )\|_{\mathcal{B}(\epsilon )}
 + \| \hat{\psi }_i(\epsilon )-\psi _i (\epsilon )
 \|_{\mathcal{B}(\epsilon )}\\
&\leq  \| \varphi_i -P_{\mathcal{H}, \mathcal{B}(\epsilon )}
\varphi_i \| _{\mathcal{H}} +\big\| P_{\mathcal{H},
\mathcal{B}(\epsilon )} \varphi_i-\sum^{k_{p+1}} _{\ell =k_p+1}
a_{i,\ell} (\epsilon ) \varphi_\ell  (\epsilon )
\big\|_{\mathcal{A}(\epsilon )}\\
&\quad + \big\| \sum^{k_{p+1}}_{\ell =k_p+1} a_{i, \ell}
(\epsilon )[\varphi_{\ell}(\epsilon )-P_{\mathcal{A}(\epsilon ),
 \mathcal{B}(\epsilon)} \varphi_\ell (\epsilon )]
\big\|_{\mathcal{A}(\epsilon )}
+ \| \hat{\psi}_i(\epsilon )-\psi_i (\epsilon )
\|_{\mathcal{B}(\epsilon )}.
\end{split}\end{equation}
Consider the term
\[
\big\| P_{\mathcal{H}, \mathcal{B}(\epsilon )} \varphi_i
-\sum^{k_{p+1}}_{\ell =k_p+1} a_{i, \ell } (\epsilon )
\varphi_\ell (\epsilon )\big\|_{\mathcal{A}(\epsilon )}
\]
in \eqref{eq:2.88}. We have
\begin{equation}\begin{split}\label{eq:2.89}
&  e^{-H(\epsilon )t} P_{\mathcal{H}, \mathcal{B}(\epsilon )} \varphi_i -P_{\mathcal{H}, \mathcal{B}(\epsilon )} e^{-Ht}\varphi_i\\
&=  \Big( \sum^{k_p}_{\ell=1} +\sum^{k_{p+1}}_{\ell =k_p+1}
+\sum^{\infty}_{\ell =k_{p+1}+1}\Big) a_{i,\ell }
(\epsilon )[e^{-\mu_\ell (\epsilon )t}
-e ^{-\mu_it}]\varphi_\ell(\epsilon ).
\end{split}\end{equation}
 By (A28) and the orthogonality of
$\{ \varphi_\ell (\epsilon )\}^\infty_{\ell =1}$,
each of the three sums in \eqref{eq:2.89} approaches $0$ as
$\epsilon \downarrow 0$. Hence, together with Theorem~\ref{thm:2.25},
we have, for $i=k_p+1,\dots ,k_{p+1}$,
\begin{equation}\label{eq:2.90}
\Big( \sum^{k_p}_{\ell =1} +\sum^\infty_{\ell=k_{p+1}+1}\Big)
a_{i,\ell}(\epsilon )^2\to 0 \quad \text{as }
\epsilon \downarrow 0.
\end{equation}
Thus, for $i=k_p+1,\dots ,k_{p+1}$,
\begin{equation}\begin{split}\label{eq:2.91}
&\lim_{\epsilon \downarrow 0}
\big\|P_{\mathcal{H}, \mathcal{B}(\epsilon )}
\varphi_i-\sum^{k_{p+1}}_{\ell =k_p+1} a_{i,\ell }
(\epsilon ) \varphi_\ell (\epsilon )\big\|^2_{\mathcal{A}(\epsilon)}\\
&= \lim_{\epsilon \downarrow 0} \Big( \sum^{k_p}_{\ell =1}
+\sum^{\infty}_{\ell =k_{p+1}+1} \Big) a_{i,\ell }(\epsilon )^2=0.
\end{split}\end{equation}
By (A9) and (A28) we have
\[
\lim_{\epsilon \downarrow 0} \| \varphi_\ell (\epsilon )
-P_{\mathcal{A}(\epsilon ), \mathcal{B}(\epsilon )}
\varphi_\ell (\epsilon )\|_{\mathcal{A}(\epsilon )}=0
\]
for all $\ell =1,2,3,\dots$. Thus
\begin{equation}\label{eq:2.92}
 \lim_{\epsilon \downarrow 0} \big\| \sum^{k_{p+1}}_{\ell =k_p+1}
a_{i,\ell } (\epsilon ) [\varphi_\ell (\epsilon )
-P_{\mathcal{A}(\epsilon ), \mathcal{B}(\epsilon )}
\varphi_\ell (\epsilon )]\big\|_{\mathcal{A}(\epsilon )}=0.
\end{equation}
By (A7) and \eqref{eq:2.91} we have, for $i=k_p+1,\dots ,k_{p+1}$,
\begin{equation}\label{eq:2.93}
\lim_{\epsilon \downarrow 0} \sum^{k_{p+1}}_{\ell =k_p+1}
a_{i,\ell }(\epsilon )^2=1.
\end{equation}
Thus, for $i=k_p+1,\dots , k_{p+1}$, \eqref{eq:2.85}, \eqref{eq:2.92}
and \eqref{eq:2.93} imply
\begin{equation}\begin{split}\label{eq:2.94}
\lim_{\epsilon \downarrow 0}
 \| \hat{\psi}_i (\epsilon )\|_{\mathcal{B}(\epsilon)}
&= \lim_{\epsilon \downarrow 0} \| \hat{\psi}_i(\epsilon )
  \|_{\mathcal{A}(\epsilon)}\\
&=\lim_{\epsilon \downarrow 0} \big\| \Big( \hat{\psi}_i (\epsilon )
  -\sum^{k_{p+1}}_{\ell =k_p+1} a_{i,\ell} (\epsilon )\varphi_\ell
 (\epsilon )\Big) +\sum^{k_{p+1}}_{\ell =k_p+1} a_{i,\ell }
 (\epsilon )\varphi_\ell (\epsilon )\big\|_{\mathcal{A}(\epsilon )}\\
&=\lim_{\epsilon \downarrow 0}
 \big\| \sum^{k_{p+1}}_{\ell =k_p+1} a_{i,\ell }
 (\epsilon )\varphi_\ell (\epsilon )\big\| _{\mathcal{A}(\epsilon )}\\
&=\lim_{\epsilon \downarrow 0}
\Big\{ \sum^{k_{p+1}}_{\ell =k_p+1} a_{i,\ell } (\epsilon )^2
 \Big\}^{1/2}
=1.
\end{split}\end{equation}
Therefore,
\begin{equation} \label{eq:2.95}
\lim_{\epsilon \downarrow 0}\| \hat{\psi}_i(\epsilon )
-\psi_i (\epsilon )\|_{\mathcal{B}(\epsilon )}
=\lim_{\epsilon \downarrow 0} |1-\| \hat{\psi}_i (\epsilon )
\|^{-1}_{\mathcal{B}(\epsilon )} |\|\hat{\psi}_i (\epsilon )
\|_{\mathcal{B}(\epsilon )}
=0.
\end{equation}
The theorem now follows from \eqref{eq:2.88}, (A7), \eqref{eq:2.91},
\eqref{eq:2.92} and \eqref{eq:2.95}.
\end{proof}


\section{Application to Neumann Laplacians on domains in
$\mathbb{R}^N$}\label{sec:3}

The purpose of this section is to show that the assumptions (A1)--(A28)
in Section~\ref{sec:2} are all satisfied when applying the abstract
theory in Section~\ref{sec:2} to the situation studied in this section.
For our application, it will be easy to check that (A1)--(A27)
are satisfied. So we shall show that (A28) holds for our application.
Throughout this section we let $\Omega \subseteq \mathbb{R}^N$
be a bounded Sobolev extension domain. Fix a sufficiently small
$\epsilon _0>0$. For each $\epsilon \in (0,\epsilon _o]$
let $\Omega_\epsilon $, $\Omega^\epsilon$ and $\Omega (\epsilon )$
be bounded Sobolev extension domains in $\mathbb{R}^N$ satisfying
\begin{equation}\label{eq:3.1}
\begin{gathered}
\Omega_\epsilon \supseteq \{ x \in \Omega :\operatorname{dist} (x ,\partial \Omega )>\epsilon \},\\
\Omega ^\epsilon \subseteq \{ x \in \mathbb{R}^N:\operatorname{dist} (x ,\Omega )<\epsilon \},\\
\Omega _\epsilon \subseteq \Omega (\epsilon )\subseteq \Omega^\epsilon .
\end{gathered}\end{equation}
We shall assume that
$\{ \Omega _\epsilon \}_{0<\epsilon \leq \epsilon_0}$ is a
decreasing family of domains in the sense that
\begin{equation}\label{eq:3.2}
\Omega_{\epsilon_1}\supseteq \Omega_{\epsilon _2}\quad \text{if }
0<\epsilon_1 \leq \epsilon _2.
\end{equation}
Similarly we shall assume that $\{\Omega^\epsilon \}_{0<\epsilon
\leq \epsilon _0}$ is an increasing family of domains in the sense
that
\begin{equation}\label{eq:3.3}
\Omega^{\epsilon _1} \subseteq \Omega^{\epsilon _2}\quad
\text{if }0<\epsilon _1\leq \epsilon_2.
\end{equation}
We shall apply the abstract theory in Section~\ref{sec:2} by putting:
\begin{equation}
\begin{gathered}
\mathcal{H}^\epsilon =L^2(\Omega^\epsilon ),\quad
\mathcal{H}_\epsilon =L^2(\Omega_\epsilon ),\quad
\mathcal{H}(\epsilon )=L^2(\Omega (\epsilon ))=\mathcal{A}(\epsilon ),
\\
\mathcal{B} (\epsilon )=L^2(\Omega \cap \Omega (\epsilon )),\quad
\mathcal{C}(\epsilon )=L^2 (\Omega (\epsilon) \backslash \Omega ),\quad
\mathcal{D}(\epsilon )=\{ 0\}.
\end{gathered}\label{eq:3.4}
\end{equation}
Let $-\Delta _\epsilon $, $-\Delta $, $-\Delta ^\epsilon$,
$-\Delta (\epsilon )$ be the Neumann Laplacian defined on
$\Omega_\epsilon $, $\Omega$, $\Omega^\epsilon$ and
$\Omega (\epsilon )$, respectively. When applying the abstract
theory in Section~\ref{sec:2} we shall put
\begin{equation}\label{eq:3.5}
 H_\epsilon =-\Delta_\epsilon ,\quad H=-\Delta ,\quad
H^\epsilon =-\Delta^\epsilon,\quad H(\epsilon )=-\Delta (\epsilon ).
\end{equation}
We shall write $P_\epsilon (t,x,y)$, $P(t,x,y)$, $P^\epsilon (t,x,y)$
and $P(\epsilon )(t,x,y)$ for the heat kernel of
$e^{\Delta _\epsilon t}$, $e^{\Delta t}$, $e ^{\Delta ^\epsilon t}$ and
$e^{\Delta (\epsilon )t}$, respectively. We shall assume that
there exists a positive continuous functions
$c:(0,1]\to (0,\infty)$ such that
\begin{equation}
\begin{gathered}
P_\epsilon (t,x,y)\leq c(t) \quad (x,y\in \Omega_\epsilon ),\\
P(t,x,y)\leq c(t) \quad (x,y\in \Omega),\\
P^\epsilon (t,x,y)\leq c(t) \quad (x,y\in \Omega^\epsilon )\\
P(\epsilon )(t,x,y) \leq c(t) \quad (x,y\in \Omega (\epsilon ))
\end{gathered}\label{eq:3.6}
\end{equation}
for all $0<\epsilon \leq \epsilon_0$ and all $0<t\leq 1$.

 We shall need the parabolic Harnack inequality:
\begin{proposition}[{\cite[Lemma 4.10]{P1}}]\label{prop:3.1}
Let $\Sigma$ be a domain in $\mathbb{R}^d$, let $u$ be a solution
of the parabolic equation:
\[
\frac{\partial u}{\partial t} -\omega^{-1} \sum^{d}_{i,j=1}
\{ \frac{\partial }{\partial x_i} ( a_{ij}
\frac{\partial u}{\partial x_j})\}=0
\]
in $\Sigma \times (\tau_1,\tau_2)$, where $\omega$ and $\{a_{ij}\}$
satisfy
\begin{gather*}
0<\lambda^{-1} \leq \omega (x)\leq \lambda <\infty \quad
  (x \in \Sigma ),\\
0<\lambda^{-1} \leq \{ a_{ij}(x )\}\leq \lambda <\infty \quad
 (x \in \Sigma),
\end{gather*}
for some $\lambda \geq 1$. Let $\Sigma '$ be a subdomain of
$\Sigma $ and suppose that
$\operatorname{dist} ( \Sigma ',  \partial \Sigma ) >\eta$  and
$ t_1-\tau _1 \geq \eta^2$.
Then
\[
|u(x ,t)-u(y,s)|\leq A[|x-y|+|t-s|^{1/2}]^{\alpha}
\]
for all $x,y\in \Sigma  '$ and $t,s\in [t_1,\tau_2)$, where
$\alpha\in (0,1]$ depends only on $d$ and $\lambda$, and
\[
A=\big( \frac{4}{\eta}\big)^\alpha \theta
\]
where $\theta$ is the oscillation of $u$ in
$\Sigma  \times (\tau _1,\tau_2)$.
\end{proposition}

\begin{theorem}\label{thm:3.2}
 We have
$\lim_{\epsilon \downarrow 0} P(\epsilon )(t,x,y)=P(t,x,y)$
for all $t\in (0,1]$ and $x,y\in \Omega$.
\end{theorem}

\begin{proof}
Suppose, for a contradiction, that for some $t_0\in (0,1]$ and
some $x_0,y_0\in \Sigma $ we have
\begin{equation}\label{eq:3.7}
P(\epsilon )(t_o,x_0,y_0) \not\to P(t_o,x_o,y_o)\quad \text{as }
\epsilon \downarrow 0.
\end{equation}
Then there exist $c_1\geq 1$ and a decreasing sequence $\{\epsilon_n\}^\infty_{n=1}$ of positive numbers such that $\epsilon _n\downarrow 0$ as $n\to \infty$ and that
\begin{equation}\label{eq:3.8}
c^{-1}_1\leq |P(\epsilon _n)(t_0,x_0,y_0)-P(t_0,x_0,y_0)|\quad
(n=1,2,3,\dots ).
\end{equation}
Applying Proposition~\ref{prop:3.1} with
\begin{equation} \label{eq:3.9}
\begin{gathered}
\Sigma =B\big( x_0,  \frac{5}{8} \operatorname{dist} (x_0,\partial \Omega)\big),\quad
\Sigma  '=B\big( x_0, \frac{1}{8} \operatorname{dist} (x_0,\partial \Omega )\big),\\
u(t,x)=P(t,x,y_0),\quad \lambda =1,\quad
\tau_1 =\frac{1}{4} t_0,\quad \tau_2=1,\quad t_1=\frac{1}{2}t_0,\\
\eta =\min\big\{ \frac{3}{8} \operatorname{dist} (x_0,\partial \Omega),
\frac{1}{2} t^{1/2}_0\big\},
\end{gathered}
\end{equation}
we obtain, for all $s,t\in (t_1,\tau _2) =(t_0/2,1)$ and all
$x \in B(x_0, \operatorname{dist} (x_0,\partial \Omega)/8)$,
\begin{equation}\label{eq:3.10}
|P(t,x,y_0)-P(s,x_0,y_0)|\leq A[|x-x_0|+|t-s|^{1/2}]^\alpha
\end{equation}
where $\alpha \in (0,1]$ depends only on $N$ and
\begin{equation}\label{eq:3.11}
 A=\big(\frac{4}{\eta}\big)^\alpha \theta\end{equation}
where
\begin{equation}\label{eq:3.12}
\theta=\sup_{\frac{1}{4}t_0\leq t\leq 1} c(t).
\end{equation}
(Hence $A$ depends only on $N$, $\operatorname{dist} (x_0,\partial \Omega)$ and $t_0$.) We may assume that, for all $n=1,2,3,\dots$, we have
\[
0<\epsilon_n<\min \{ \frac{3}{8}\operatorname{dist} (x_0,\partial \Omega),
\frac{3}{8} \operatorname{dist} (y_0,\partial \Omega)\}.
\]
By a similar argument we deduce that
\begin{equation}\label{eq:3.13}
|P(\epsilon_n)(t,x,y_0)-P(\epsilon_n)(s,x_0,y_0) |
\leq A[|x-x_0|+|t-s|^{1/2} ]^\alpha
\end{equation}
for all $s, t\in (t_1,\tau_2) =(  t_0/2,1)$, all
$x\in B(x_0, \operatorname{dist} (x_0,\partial \Omega)/8)$ and all $n=1,2,3,\dots $,
and where $\alpha $ and $A$ in \eqref{eq:3.13} have the same values
as those in \eqref{eq:3.10}. Let
\begin{equation}\label{eq:3.14}
R=\min\big\{ (4Ac_1)^{-\frac{1}{\alpha}},\frac{1}{8}
\operatorname{dist} (x_0,\partial \Omega )\big\}.
\end{equation}
Then, for all $x\in B (x_0,R)$, $t\in (t_0/2,1)$ and
$n=1,2,3,\dots $, we have
\begin{gather}\label{eq:3.15}
|P(t,x,y_0)-P(t,x_0,y_0)|\leq (4c_1)^{-1},\\
\label{eq:3.16}
|P(\epsilon_n)(t,x,y_0)-P(\epsilon _n)(t,x_0,y_0)|\leq (4c_1)^{-1}.
\end{gather}
For $x\in B(x_0,R)$ and $n=1,2,3,\dots $ we have
\begin{equation}\begin{split}\label{eq:3.17}
&|P(\epsilon _n)(t_0,x_0,y_0)-P(t_0,x_0,y_0)|\\
&\leq  |P(\epsilon_n) (t_0,x_0,y_0)-P(\epsilon_n)(t_0,x,y_0)|
+|P(\epsilon _n)(t_0,x,y_0)-P(t_0,x,y_0)|\\
&\quad +|P(t_0,x,y_0)-P(t_0,x_0,y_0)|.
\end{split}\end{equation}
So, by \eqref{eq:3.8}, \eqref{eq:3.15}, \eqref{eq:3.16} and
\eqref{eq:3.17}, we obtain
\begin{equation}\label{eq:3.18}
\frac{1}{2} c^{-1}_1 \leq |P(\epsilon _n)(t_0,x,y_0)-P(t_0,x,y_0)|
\end{equation}
for all $x\in B(x_0,R)$ and $n=1,2,3,\dots $.
Integrating \eqref{eq:3.18} over $B(x_0,R)$ we obtain
\begin{equation}\begin{split}\label{eq:3.19}
&\frac{1}{2} c^{-1}_1 |B(x_0,R)|\\
&\leq \Big|\int_{\Omega }P(t_0 ,x,y_0)1_{B(x_0,R)} (x) \,dx
 -\int_{\Omega (\epsilon_n)} P(\epsilon _n)(t_0,x,y_0)
1_{B(x_0,R)}(x)\, dx\Big|.
\end{split}
\end{equation}
Put
\[
u(t,y)=\int_\Omega P(t,x,y)1_{B(x_0,R)} (x)\, dx
\]
and, for $n=1,2,3,\dots $, put
\[
u_n(t,y)=\int_{\Omega (\epsilon _n)}
P(\epsilon _n)(t,x,y)1_{B(x_0,R)} (x)\, dx.
\]
Then $u(t,y)$ and $u_n(t,y)$ satisfy the parabolic equations
\begin{gather*}
\frac{\partial u}{\partial t} =\Delta u \quad\text{in }
(0,1)\times \Omega,\\
\frac{\partial u_n}{\partial t} =\Delta u_n \quad \text{in }
(0,1)\times \Omega (\epsilon _n),
\end{gather*}
respectively. So we can apply the parabolic Harnack inequality
(Proposition~\ref{prop:3.1}) to $u(t,y)$ and $u_n(t,y)$ and,
as in \eqref{eq:3.10} and \eqref{eq:3.13}, obtain
\begin{equation}\label{eq:3.20}
|u(t,y)-u(s,y_0)|\leq \tilde{A}[|y-y_0|
+|t-s|^{1/2}|^{\tilde{\alpha}}
\end{equation}
for all $y\in B(y_0,\operatorname{dist} (y_0,\partial\Omega)/8)$ and
$t,s\in (t_0/2,1)$, and
\begin{equation}\label{eq:3.21}
|u_n(t,y)-u_n(s,y_0)|\leq \tilde{A}[|y-y_0|+|t-s|^{1/2}]
^{\tilde{\alpha}}
\end{equation}
for all $y\in B(y_0,\operatorname{dist} (y_0,\partial \Omega )/8)$ and
$t,s\in (t_0/2,1)$ where $\tilde{\alpha}\in (0,1]$ depends only
on $N$ and
\[
\tilde{A}=\big(\frac{4}{\tilde{\eta}} \big)^{\tilde{\alpha}}
\tilde{\theta}\leq \big(\frac{4}{\tilde{\eta}}\big)^{\tilde{\alpha}}
\]
where
\[
\tilde{\eta} = \min\{\frac{3}{8}\operatorname{dist} (y_0,\partial \Omega ),
\frac{1}{2}t_0^{1/2}\}
\]
 and
\begin{align*}
\tilde{\theta} &=\sup \big\{ \frac{1}{4} t_0\leq t\leq 1, |y-y_0|
\leq \frac{5}{8} \operatorname{dist} (y_0,\partial \Omega): u(t,y)\big\}\\
&\leq \sup \big\{ \frac{1}{4} t_0 \leq t\leq 1, \,|y-y_0|
 \leq \frac{5}{8} \operatorname{dist} (y_0,\partial \Omega ):
 \int_\Omega P(t,x,y)\,dx\big\}
\leq 1.
\end{align*}
(Hence $\tilde{A}$ depends only on $N$, $t_0$ and
$\operatorname{dist}(y_0,\partial \Omega)$.) Let
\[
\tilde{R} =\min\big\{ \big[ \frac{1}{8} |B(x_0,R)
|c^{-1}_1 \tilde{A}^{-1} \big]^{\frac{1}{\tilde{\alpha}}} ,
\frac{1}{8} \operatorname{dist} (y_0,\partial \Omega )\big\}.
\]
Then, by \eqref{eq:3.20} and \eqref{eq:3.21},
\begin{gather}\label{eq:3.22}
|u(t_0,y)-u(t_0,y_0)|\leq \frac{1}{8} |B(x_0,R)|c^{-1}_1,\\
\label{eq:3.23}
|u_n (t_0,y)-u_n(t_0,y_0)|\leq \frac{1}{8} |B(x_0,R)|c^{-1}_1
\end{gather}
for all $y\in B(y_0,\tilde{R}$). Thus, for all
$y\in B(y_0,\tilde{R})$, we have
\begin{equation}\begin{split}\label{eq:3.24}
&|u_n(t_0,y_0)-u(t_0,y_0)|\\
&\leq  |u_n(t_0,y_0)-u_n(t_0,y)|+|u_n(t_0,y)-u(t_0,y)|
 + |u(t_0,y)-u(t_0,y_0)|\\
&\leq  \frac{1}{4} |B(x_0,R)|c^{-1}_1 + |u_n(t_0,y)-u(t_0,y)|.
\end{split}\end{equation}
So, by \eqref{eq:3.19} and \eqref{eq:3.24}, we have
\begin{equation}\label{eq:3.25}
 \frac{1}{4} |B(x_0,R)|c^{-1}_1 \leq |u_n(t_0,y)-u(t_0,y)|
\end{equation}
for all $y\in B(y_0,\tilde{R})$. But
\[
u_n(t_0,y)= \int_{\Omega (\epsilon _n)} P(\epsilon _n)
 (t_0,x,y)1_{B(x_0,R)} (x)\,dx
=(e^{-H(\epsilon _n)t_0} \, 1_{B(x_0,R)})(y)
\]
and
\[
 u(t_0,y)= \int_\Omega P(t_0,x,y)1_{B(x_0,R)} (x)\,dx
=(e^{-Ht_0} \, 1_{B(x_0,R)})(y).
\]
Thus \eqref{eq:3.25} implies
\begin{align*}
&\int_{B(y_0,\tilde{R})} |(e^{-H(\epsilon _n)t_0} 1_{B(x_0,R)} )(y)-(e^{-Ht_0}1_{B(x_0,R)})(y)|^2\,dy\\
& \geq \frac{1}{16} c^{-2}_1 |B(x_0,R)|^2 |B(y_0,\tilde{R})|,
\end{align*}
hence, for all $n=1,2,3,\dots$,
\begin{equation}\begin{split}\label{eq:3.26}
&\|e^{-H(\epsilon _n)t_0} 1_{B(x_0,R)} - e^{-Ht_0} 1_{B(x_0,R)} \|^2_{L^2(B(y_0,\tilde{R}))}\\
&\geq  \frac{1}{16} c^{-2}_1 |B(x_0,R)|^2|B(y_0,\tilde{R})|.
\end{split}\end{equation}
Let $f\in L^2(\Omega^{\epsilon_0})$ be the function defined by
\[
f(y)=\begin{cases} 1 &\text{if } |y-x_0|<R\\
0 &  \text{if } y\in \Omega^{\epsilon_0} \text{ and } |y-x_0|\geq R.
\end{cases}
\]
By Theorem~\ref{thm:2.17} we have, for all $n=1,2,3,\dots $,
\[
\lim_{\epsilon \downarrow 0} \|e^{-\hat{H}(\epsilon )t_0} f
- e^{-\hat{H}t_0} f\|_{L^2 (B(y_0,\tilde{R}))}
\leq  \lim_{\epsilon \downarrow 0} \| e^{-\hat{H}(\epsilon)t_0}
f- e^{-\hat{H}t_0} f\|_{L^2(\Omega ^{\epsilon _0})}
=  0,
\]
thus
\[
\lim_{\epsilon \downarrow 0} \int_{B(y_0,\tilde{R})}
|(e^{-\tilde{H}(\epsilon )t_0} f)(y)-(e^{-\hat{H}t_0}f)(y)|^2\, dy=0
\]
and hence
\[
\lim_{\epsilon \downarrow 0} \int_{B(y_0,\tilde{R})}
|(e^{-H(\epsilon )t_0}1_{B(x_0,R)} )(y)
-(e^{-Ht} 1_{B(x_0,R)} )(y)|^2 \, dy=0.
\]
But this implies
\[
\lim_{n\to \infty} \| e^{-H(\epsilon _n)t_0} 1_{B(x_0,R)}
- e^{-Ht_0} 1_{B(x_0,R)} \|^2_{L^2(B(y_0,\tilde{R}))}=0
\]
which contradicts \eqref{eq:3.26}. Therefore
 assumption \eqref{eq:3.7} must be false and the theorem is proved.
\end{proof}

 We now show that the first equality of the assumption (A28)
is satisfied. We note that for any $f\in \mathcal{H}=L^2 (\Omega)$.
\[
P_{\mathcal{H}, \mathcal{B}(\epsilon)}f
=P_{L^2(\Omega), L^2(\Omega \cap \Omega (\epsilon ))}  f
=1_{\Omega \cap \Omega (\epsilon )} f.
\]
Thus for all $\epsilon \in (0,\epsilon_0]$,
$x\in \Omega(\epsilon)$ and $n=1,2,3,\dots$,
\begin{equation}\begin{split}\label{eq:3.27}
&[P_{\mathcal{H}, \mathcal{B}(\epsilon)} e^{-Ht} \varphi_n-e^{-H(\epsilon )t} P_{\mathcal{H}, \mathcal{B}(\epsilon)} \varphi_n](x)\\
&=  1_{\Omega \cap \Omega (\epsilon)} (x)
 \int_{\Omega} P(t,x,y)\varphi_n(y)\, dy
 -  \int_{\Omega(\epsilon)} P(\epsilon )(t, x, y)1_{\Omega \cap
  \Omega (\epsilon)} (y) \varphi_n (y)\, dy\\
&=   1_{\Omega \cap \Omega (\epsilon) } (x)
\Big( \int_{\Omega \backslash \Omega (\epsilon)}
 +\int_{\Omega \cap \Omega (\epsilon)} \Big)
  P(t,x,y)\varphi _n(y)\, dy\\
&\quad -  \Big( \int_{\Omega (\epsilon )\backslash \Omega }
 +\int_{\Omega \cap \Omega (\epsilon)} \Big)
 P(\epsilon )(t, x, y)1_{\Omega \cap \Omega (\epsilon)}
 (y)\varphi_n (y)\, dy\\
&=  1_{\Omega \cap \Omega (\epsilon)} (x)\int_{\Omega \backslash \Omega (\epsilon)} P(t,x,y)\varphi_n(y)\, dy\\
& +  \int_{\Omega \cap \Omega (\epsilon)} 1_{\Omega \cap \Omega (\epsilon)} (x) P(t,x,y)\varphi_n (y)
 -  P(\epsilon )(t,x,y)1_{\Omega \cap \Omega (\epsilon)}
(y)\varphi_n(y)\, dy
\end{split}\end{equation}
since
\[
\int_{\Omega (\epsilon)\backslash \Omega} P(\epsilon)(t,x,y)
1_{\Omega \cap \Omega (\epsilon)} (y)\varphi_n(y)\, dy=0.
\]

Let $B$ be a ball such that
$ B\subseteq \Omega_\epsilon$ $(0<\epsilon \leq \epsilon_0)$.
For each $k=1,2,3,\dots $ let $\lambda_k (\epsilon)$ and
$\lambda_k(B)$ be the $k$-th eigenvalue of the Dirichlet Laplacian
defined on $\Omega (\epsilon )$ and $B$, respectively. Then,
by min-max,
\begin{equation}\label{eq:3.28}
\mu_k(\epsilon )\leq \lambda_k (\epsilon) \leq \lambda_k(B).
\end{equation}
By the assumption \eqref{eq:3.6}, we have
\[
\sum^\infty_{k=1} e^{-\mu_k(\epsilon )t} \varphi_k(\epsilon)(x)^2
\leq c(t)
\]
for all $0<t\leq 1$, $0<\epsilon \leq \epsilon_0$ and
$x\in \Omega (\epsilon)$.
Hence
\begin{equation}\label{eq:3.29}
|\varphi_k(\epsilon )(x)|\leq [c(t)e^{\mu_k(\epsilon)t}]^{1/2}
\leq c(t)^{1/2} e^{\lambda_k(B)t/2}
\end{equation}
for all $0<\epsilon \leq \epsilon_0$, $x\in\Omega (\epsilon)$,
$0<t\leq 1$ and $k=1,2,3,\dots$. Similarly we have
\begin{equation}\label{eq:3.30}
|\varphi_k(x)|\leq c(t)^{1/2}e^{\lambda_k(B) t/2}
\end{equation}
for all $0<t\leq 1$, $x\in \Omega$ and $k=1,2,3,\dots $. Since
\[
|\Omega \backslash \Omega (\epsilon)|\leq |\Omega \backslash
\Omega_\epsilon |\to 0\quad \text{as } \epsilon \downarrow 0,
\]
we have, for all $0<t \leq 1$,
\begin{equation} \label{eq3.31}
|1_{\Omega \cap \Omega (\epsilon)} (x)
 \int_{\Omega \backslash \Omega (\epsilon)} P(t,x,y)\varphi_n(y)\,dy|
\leq  c(t) |\Omega \backslash\Omega (\epsilon)|c(1)^{1/2}
e^{\lambda_n(B)/2}
\to  0 \quad\text{as } \epsilon \downarrow 0\,.
\end{equation}
Next we consider the term
\[
\int_{\Omega \cap \Omega (\epsilon)} [1_{\Omega
\cap \Omega (\epsilon)} (x)P(t,x,y)-P(\epsilon )(t,x,y)]\varphi_n(y)\,dy
\]
in \eqref{eq:3.27}. Let $0<\epsilon_1<\epsilon_0$.
For $0<\epsilon \leq \epsilon_1$, $x\in \Omega \cap \Omega (\epsilon)$
and $n=1,2,3,\dots $,  by \eqref{eq:3.30}, we have
\begin{equation}\begin{split}\label{eq:3.32}
&\Big| \int_{\Omega \cap \Omega (\epsilon) }
[1_{\Omega \cap \Omega (\epsilon)} (x)
 P(t,x,y)-P(\epsilon )(t,x,y)]\varphi _n(y) \, dy\Big|\\
&\leq  \int_{\Omega \cap \Omega (\epsilon)} |P(t,x,y)-P(\epsilon )(t,x,y)||\varphi_n(y)|\, dy\\
&\leq  c(1)^{1/2} e^{\lambda_n(B)/2} \int_{\Omega \cap \Omega(\epsilon)} |P(t,x,y)-P(\epsilon )(t,x,y)|\, dy\\
&\leq  c(1)^{1/2} e^{\lambda_n(B)/2}
 \Big\{ \int_{(\Omega \cap \Omega (\epsilon ))\backslash
 \Omega_{\epsilon_1}} |P(t,x,y)-P(\epsilon )(t,x,y)|\, dy \\
& \quad+\int_{\Omega _{\epsilon_1}} |P(t,x,y)-P(\epsilon) (t,x,y)|\,dy
 \Big\}\\
&\leq  c(1)^{1/2} e^{\lambda_n(B)/2} \{ |\Omega^{\epsilon_1}
 \backslash \Omega_{\epsilon_1} |2c(t)
+\int_{\Omega_{\epsilon_1}} |P(t,x,y)-P(\epsilon)(t,x,y)|\, dy\Big\}.
\end{split}
\end{equation}
For $x\in \Omega (\epsilon)\backslash \Omega$, $0<t\leq 1$ and
$n=1,2,3,\dots$, we have
\begin{equation}\begin{split}\label{eq:3.33}
&\Big| \int_{\Omega \cap \Omega (\epsilon)} [1_{\Omega
 \cap \Omega (\epsilon)} (x)P(t,x,y)-P(\epsilon) (t,x,y)]\varphi_n(y)
 \,dy\Big|\\
&=   \int _{\Omega \cap\Omega (\epsilon)} P(\epsilon)(t,x,y)\varphi_n (y)\, dy\\
&\leq    |\Omega \cap \Omega (\epsilon)|c(t) c(1)^{1/2}
e^{\lambda_n (B)/2}.
\end{split}\end{equation}
For every $0<t\leq 1$, $0<\epsilon \leq \epsilon_0$ and
$n=1,2,3,\dots$,
\begin{equation}\begin{split}\label{eq:3.34}
&  \int_{\Omega (\epsilon)} |(P_{\mathcal{H}, \mathcal{B} (\epsilon)} e^{-Ht} \varphi_n - e^{-H(\epsilon )t} P_{\mathcal{H}, \mathcal{B}(\epsilon)} \varphi_n)(x)|^2 \, dx\\
&=   \int_{\Omega (\epsilon)\backslash \Omega }
 |(P_{\mathcal{H}, \mathcal{B}(\epsilon)} e^{-Ht} \varphi_n
 - e^{-H(\epsilon )t}P_{\mathcal{H}, \mathcal{B}(\epsilon)}
 \varphi_n)(x)|^2\, dx\\
&\quad  + \int_{\Omega (\epsilon)\cap \Omega}
 |(P_{\mathcal{H}, \mathcal{B}(\epsilon)} e^{-Ht}\varphi_n
 - e^{-H(\epsilon)t} P_{\mathcal{H}, \mathcal{B}(\epsilon)} \varphi_n)
 (x)|^2 \, dx.
\end{split}\end{equation}
For the first term on the right side of \eqref{eq:3.34} we have,
 by \eqref{eq:3.27}, \eqref{eq:3.30} and \eqref{eq:3.33},
\begin{equation}\begin{split}\label{eq:3.35}
& \int_{\Omega (\epsilon )\backslash \Omega} |(P_{\mathcal{H},
 \mathcal{B}(\epsilon)} e^{-Ht} \varphi_n
 - e^{-H(\epsilon)t} P_{\mathcal{H}, \mathcal{B}(\epsilon)}
 \varphi_n )(x)|^2\, dx\\
 &\leq  |\Omega^\epsilon\backslash \Omega |\{ |\Omega \cap
\Omega (\epsilon) |c(t)c(1)^{1/2}e^{\lambda_n(B)/2}\}^2
 \to   0 \quad \text{as } \epsilon \downarrow 0.
\end{split}\end{equation}

 Next we consider the second term on the right side of \eqref{eq:3.34}.
For $t\in (0,1]$, $n=1,2,3,\dots$ and $\epsilon \in (0,\epsilon_0]$
let $F_{t,n,\epsilon}:\Omega \to \mathbb{R}$ be defined by
\begin{equation}\label{eq:3.36}
 F_{t,n,\epsilon} (x)=\begin{cases}
0 & \text{if } x\in \Omega \backslash \Omega (\epsilon)\\
|(P_{\mathcal{H},\mathcal{B}(\epsilon)} e^{-Ht} \varphi_n
 - e^{-H(\epsilon )t} P_{\mathcal{H},
  \mathcal{B}(\epsilon)} \varphi_n)(x)|^2
& \text{if } x\in \Omega \cap \Omega (\epsilon).
\end{cases}\end{equation}
If $0<\epsilon \leq \epsilon_1\leq \epsilon_0$ and
$x\in \Omega \cap \Omega (\epsilon)$, then
\begin{equation}\begin{split}\label{eq:3.37}
F_{t,n,\epsilon} (x)
&\leq \{|\Omega \backslash \Omega (\epsilon) |c(t)c(1)^{1/2}
 e^{\lambda_n(B)/2}
  +c(1)^{1/2} e^{\lambda_n(B)/2} [|\Omega \backslash
 \Omega_{\epsilon_1} |2c(t)\\
&\quad +\int_{\Omega_{\epsilon_1}} |P(t,x,y)
 -P(\epsilon )(t,x,y) |\, dy]\}^2.
\end{split}\end{equation}
For fixed $t\in (0,1]$, $n=1,2,3,\dots $ and $x\in \Omega$,
given any $\delta >0$ we can first choose
$\epsilon_1\in (0,\epsilon_0]$ such that
\[
c(1)^{1/2} e^{\lambda_n(B)/2} |\Omega \backslash
\Omega _{\epsilon_1} |2c(t)\leq \delta /2,
\]
then, by Theorem~\ref{thm:3.2}, we can choose
$\epsilon_2\in (0,\epsilon_1]$ such that
\[
c(1)^{1/2}e^{\lambda_n (B)/2} \int_{\Omega_{\epsilon _1}}
|P(t,x,y)-P(\epsilon )(t,x,y)|\, dy\leq \delta/2
\]
for all $\epsilon \in (0,\epsilon_2]$. Thus for all
$t\in (0,1]$, $n=1,2,3,$ $\dots $ and $x\in \Omega$, we have
\begin{equation}\label{eq:3.38}
\lim_{\epsilon \downarrow 0} F_{t,n,\epsilon} (x)=0.
\end{equation}
From \eqref{eq:3.37} we see that
\begin{equation}\label{eq:3.39}
F_{t,n,\epsilon} (x)\leq [c(1)^{1/2} e^{\lambda_n(B)/2} 5c(t)
|\Omega |]^2
\end{equation}
for all $t\in (0,1]$, $n=1,2,3,\dots$, $\epsilon \in (0,\epsilon_0]$
and $x\in \Omega$. Therefore, by \eqref{eq:3.38}, \eqref{eq:3.39}
and the dominated convergence theorem, we have
\begin{equation}\begin{split} \label{eq:3.40}
& \lim_{\epsilon \downarrow 0} \int_{\Omega \cap
 \Omega (\epsilon)} |(P_{\mathcal{H}, \mathcal{B}(\epsilon)}
 e^{-Ht} \varphi_n - e^{-H(\epsilon )t}P_{\mathcal{H}, \mathcal{B}
 (\epsilon)} \varphi_n)(x)|^2\, dx\\
&= \lim_{\epsilon\downarrow 0} \int_\Omega F_{t,n,\epsilon} (x)\, dx
=  0
\end{split}\end{equation}
for all $t\in (0,1]$ and $n=1,2,3,\dots$. So
\begin{equation}\begin{split}\label{eq:3.41}
&  \| P_{\mathcal{H}, \mathcal{B}(\epsilon)} e^{-Ht} \varphi_n -e^{-H(\epsilon )t}P_{\mathcal{H}, \mathcal{B}(\epsilon)} \varphi_n\|^2_{\mathcal{A}(\epsilon)}\\
&=   \int_{\Omega (\epsilon)} |(P_{\mathcal{H}, \mathcal{B}(\epsilon)} e^{-Ht}\varphi_n- e^{-H(\epsilon)t} P_{\mathcal{H}, \mathcal{B}(\epsilon)} \varphi_n)(x)|^2\, dx\\
&=   \int_{\Omega (\epsilon )\backslash \Omega} |(P_{\mathcal{H}, \mathcal{B}(\epsilon )} e^{-Ht} \varphi_n- e^{-H(\epsilon )t} P_{\mathcal{H}, \mathcal{B}(\epsilon)} \varphi_n)(x)|^2\, dx\\
&\quad  + \int_{\Omega (\epsilon)\cap \Omega} |(P_{\mathcal{H}, \mathcal{B}(\epsilon)} e^{-Ht}\varphi_n - e^{-H(\epsilon )t} P_{\mathcal{H}, \mathcal{B}(\epsilon )} \varphi_n )(x)|^2\, dx\\
 &\leq   |\Omega (\epsilon )\backslash \Omega |\{ |\Omega \cap \Omega (\epsilon) |c(t)c(1)^{1/2}e^{\lambda_n (B)/2}\}^2\\
&\quad  +\int_{\Omega (\epsilon )\cap \Omega} |(P_{\mathcal{H}, \mathcal{B}(\epsilon)} e^{-Ht} \varphi_n- e^{-H(\epsilon )t} P_{\mathcal{H}, \mathcal{B}(\epsilon)} \varphi_n )(x)|^2\, dx\\
&\to   0 \quad \text{as } \epsilon \downarrow 0
\end{split}\end{equation}
where we have used \eqref{eq:3.27}, \eqref{eq:3.33}
 and \eqref{eq:3.40}. Hence the first equality in (A28) holds
in this application.

 We next consider the second equality in (A28).
For $x\in \Omega$, $t\in (0,1]$ and $n=1,2,3,\dots $ we have
\begin{equation}\begin{split}
&  (e^{-Ht} P_{\mathcal{A}(\epsilon ), \mathcal{B}(\epsilon )} \varphi_n (\epsilon) -P_{\mathcal{A}(\epsilon), \mathcal{B}(\epsilon)} e^{-H(\epsilon )t} \varphi_n (\epsilon) )(x)\\
&=   \int_{\Omega \cap \Omega (\epsilon)} P(t,x,y)\varphi_n (\epsilon)
(y)\, dy-1_{\Omega \cap \Omega (\epsilon)} (x)
 f_{t,n,\epsilon} (x)
\end{split}\end{equation}
where
\begin{equation}\label{eq:3.43}
f_{t,n,\epsilon} (x)=\begin{cases}
0 &\text{if } x\in \Omega \backslash \Omega (\epsilon)\\
\int_{\Omega (\epsilon)} P(\epsilon) (t,x,y)\varphi_n
(\epsilon)(y)\, dy&\text{if } x\in \Omega \cap \Omega (\epsilon).
\end{cases}\end{equation}
So for $x\in \Omega \backslash \Omega (\epsilon )$,
$t\in (0,1]$, $n=1,2,3,\dots$ and $\epsilon \in (0,\epsilon_0]$,
 by \eqref{eq:3.30}, we have
\begin{equation}\begin{split}\label{eq:3.44}
&  |(e^{-Ht} P_{\mathcal{A}(\epsilon), \mathcal{B}(\epsilon)}
 \varphi_n (\epsilon) -P_{\mathcal{A}(\epsilon),
 \mathcal{B}(\epsilon)} e^{-H(\epsilon )t} \varphi_n (\epsilon)) (x)|\\
&=   \Big|\int_{\Omega \cap \Omega (\epsilon)}
 P(t,x,y)\varphi_n(\epsilon )(y)\, dy\Big|\\
&\leq   |\Omega \cap \Omega (\epsilon)|c(t)c(1)^{1/2}
 e^{\lambda_n(B)/2}.
\end{split}\end{equation}
For $t\in (0,1]$, $n=1,2,3,\dots $ and $\epsilon \in (0,\epsilon_0]$
we define $G_{t,n,\epsilon}: \Omega \to \mathbb{R}$ by
\begin{equation}\label{eq:3.45}
G_{t,n,\epsilon} (x)=\begin{cases} 0
 &\text{if } x\in \Omega \backslash \Omega (\epsilon)\\
|(e^{-Ht} P_{\mathcal{A}(\epsilon ), \mathcal{B}(\epsilon)} \varphi_n
 (\epsilon)-P_{\mathcal{A}(\epsilon), \mathcal{B}(\epsilon)}
 e^{-H(\epsilon )t} \varphi_n(\epsilon ))(x)|
&\text{if } x\in \Omega \cap \Omega (\epsilon).
\end{cases}
\end{equation}
If $0<\epsilon \leq \epsilon_1\leq \epsilon_0$ and
$x\in \Omega \cap \Omega (\epsilon)$, then
\begin{equation}\begin{split}\label{eq:3.46}
G_{t,n,\epsilon} (x)
&= \Big| \int_{\Omega \cap \Omega (\epsilon)}
 [P(t,x,y)-P(\epsilon )(t,x,y)]\varphi_n(\epsilon) (y)\, dy\\
&\quad - \int_{\Omega (\epsilon)\backslash \Omega}
 P(\epsilon )(t,x,y)\varphi_n (\epsilon )(y)\, dy\Big|\\
&\leq \Big| \int_{(\Omega \cap \Omega (\epsilon))\backslash
 \Omega_{\epsilon_1}} [P(t,x,y)-P(\epsilon)(t,x,y)]
 \varphi_n (\epsilon)(y)\, dy\Big|\\
&\quad + \Big| \int_{\Omega_{\epsilon_1}} [P(t,x,y)
 -P(\epsilon) (t,x,y)]\varphi_n (\epsilon) (y)\, dy\Big|\\
&\quad + \Big| \int_{\Omega (\epsilon )\backslash \Omega}
 P(\epsilon )(t,x,y)\varphi_n (\epsilon )(y) \, dy\Big|\\
&\leq c(1)^{1/2} e^{\lambda_n(B)/2} \{ |\Omega^{\epsilon_1}
 \backslash \Omega_{\epsilon_1} |3c(t)\\
&\quad +\int_{\Omega_{\epsilon_1}} |P(t,x,y)
 -P(\epsilon )(t,x,y)|\, dy\}.
\end{split}\end{equation}
Thus, for fixed $t\in (0,1]$, $n=1,2,3,\dots$ and $x\in \Omega$,
given any $\delta >0$ we can first choose
$\epsilon_1\in (0,\epsilon_0]$ such that
\[
 c(1)^{1/2} e^{\lambda_n (B)/2} |\Omega^{\epsilon_1}
  \backslash \Omega_{\epsilon_1} |3c(t) \leq \delta /2,
\]
then, by Theorem~\ref{eq:3.2}, we can find
$\epsilon_2\in (0,\epsilon_1]$ such that
\[
c(1)^{1/2} e^{\lambda_n(B)/2} \int_{\Omega _{\epsilon_1}}
 |P(t,x,y)-P(\epsilon )(t,x,y)|\, dy\leq \delta /2
\]
for all $\epsilon \in (0,\epsilon_2]$. Therefore, for all
$t\in (0,1]$, $n=1,2,3,\dots $ and $x\in \Omega$, we have
\begin{equation}\label{eq:3.47}
\lim_{\epsilon\downarrow 0} G_{t,n,\epsilon} (x)=0.
\end{equation}
Also, from \eqref{eq:3.46}, we have, for all $t\in (0,1]$,
$n=1,2,3,\dots$, $\epsilon \in (0,\epsilon_0]$ and $x\in\Omega$,
\begin{equation}\label{eq:3.48}
G_{t,n,\epsilon} (x)\leq c(1)^{1/2}e^{\lambda_n(B)/2} 5c(t)
|\Omega^{\epsilon_0}|.
\end{equation}
Hence we have
\begin{equation}\begin{split}\label{eq:3.49}
&  \lim_{\epsilon \downarrow 0} \int_{\Omega \cap \Omega (\epsilon)} |(e^{-Ht} P_{\mathcal{A}(\epsilon), \mathcal{B}(\epsilon)} \varphi_n (\epsilon)-P_{\mathcal{A}(\epsilon), \mathcal{B}(\epsilon)} e^{-H(\epsilon)t} \varphi_n (\epsilon))(x)|^2\, dx\\
&=   \lim_{\epsilon\downarrow 0} \int_\Omega G_{t,n,\epsilon} (x)^2
 \, dx
=   0
\end{split}\end{equation}
for all $t\in (0,1]$ and $n=1,2,3,\dots$, using \eqref{eq:3.45},
\eqref{eq:3.47}, \eqref{eq:3.48} and the dominated convergence
theorem. So, for all $t\in (0,1]$ and $n=1,2,3,\dots$, we have
\begin{align*}
&  \| e^{-Ht} P_{\mathcal{A}(\epsilon), \mathcal{B}(\epsilon)} \varphi_n(\epsilon) -P_{\mathcal{A}(\epsilon ), \mathcal{B}(\epsilon)} e^{-H(\epsilon)t} \varphi_n(\epsilon)\|^2_{\mathcal{H}}\\
&=   \int_\Omega |(e^{-Ht} P_{\mathcal{A}(\epsilon), \mathcal{B}(\epsilon)}\varphi_n(\epsilon) -P_{\mathcal{A}(\epsilon), \mathcal{B}(\epsilon)}e^{-H(\epsilon)t} \varphi_n(\epsilon))(x)|^2\, dx\\
&=   \Big( \int_{\Omega \backslash \Omega (\epsilon)}
 +\int_{\Omega \cap \Omega (\epsilon)} \Big)
|(e ^{-Ht} P_{\mathcal{A}(\epsilon), \mathcal{B}(\epsilon)} \varphi_n (\epsilon) -P_{\mathcal{A}(\epsilon ), \mathcal{B}(\epsilon)} e^{-H(\epsilon )t} \varphi_n(\epsilon)) (x)|^2 \, dx\\
&\leq   |\Omega \backslash \Omega (\epsilon)|(|\Omega \cap \Omega (\epsilon)|c(t) c(1)^{1/2} e^{\lambda_n (B)/2})^2\\
&\quad +\int_{\Omega \cap \Omega (\epsilon)} |(e^{-Ht} P_{\mathcal{A}(\epsilon), \mathcal{B}(\epsilon)} \varphi_n (\epsilon) -P_{\mathcal{A}(\epsilon ), \mathcal{B}(\epsilon) }e^{-H(\epsilon)t} \varphi_n(\epsilon))(x)|^2\, dx\\
&\to   0 \quad \text{as } \epsilon \downarrow 0
\end{align*}
where we have used \eqref{eq:3.44} and \eqref{eq:3.49}.
Hence the second equality of (A28) holds in this application.


 Finally we consider the third equality in (A28).
For $\epsilon \in (0,\epsilon_0]$ and $n=1,2,3,\dots $ we have
\[
\varphi_n (\epsilon)=1_{\Omega (\epsilon)\backslash \Omega}
\varphi_n (\epsilon) +1_{\Omega (\epsilon)\cap \Omega}
\varphi_n (\epsilon).
\]
By \eqref{eq:3.30} we have
\[
\int_{\Omega (\epsilon)\backslash \Omega}
|\varphi _n(\epsilon )(x)|^2 \, dx
\leq |\Omega^\epsilon \backslash \Omega |c(1) e^{\lambda_n (B)}
\to 0 \quad \text{as }\epsilon \downarrow 0.
\]
Since $\| \varphi_n(\epsilon) \|^2_{\mathcal{A}(\epsilon)} =1$,
we must have
\[
\| P_{\mathcal{A}(\epsilon ), \mathcal{B}(\epsilon)}
\varphi_n (\epsilon) \|^2_{\mathcal{H}}
=\int_{\Omega \cap \Omega (\epsilon )} |\varphi_n(\epsilon )(x)|^2
\, dx
\to 1\quad \text{as } \epsilon \downarrow 0,
\]
hence the third equality of (A28) holds in this application.

\begin{theorem}\label{thm:3.3}
We use the notation in Section~\ref{sec:2}. In particular,
we shall use the notation in Definition~\ref{def:2.21} and
Theorem~\ref{thm:2.26}. Let $K$ be a compact subset of $\Omega$.
Then we have
\begin{equation}\label{eq:3.50}
\lim_{\epsilon \downarrow 0}
\big\{ \sup_{x\in K} |\varphi_i (x)-\psi_i (\epsilon) (x)|\big\}=0
\end{equation}
for all $i=1,2,3,\dots $.
\end{theorem}

\begin{proof}
We  need to consider only $i\geq 2$.
Let $p\geq 1$ be an integer and let
\[
k_p+1\le i\leq k_{p+1}.
\]
We assume, for a contradiction, that \eqref{eq:3.50} is false.
Then there exist $\delta >0$ and a decreasing sequence
$\{ \epsilon_m\}^\infty_{m=1}$  in
$( 0,\epsilon_0/2]$, with $\lim_{m\to \infty} \epsilon_m=0$,
and a sequence of points $\{ x_m\}^\infty_{m=1}$ in $K$ such that
\begin{equation}\label{eq:3.51}
|\varphi_i (x_m)-\psi_i(\epsilon_m)(x_m)|\geq \delta \quad
(m=1,2,3,\dots ).
\end{equation}
We can choose $\hat{\epsilon}\in (0,\min \{1,\epsilon_0\})$ such that
\[
 D=\{ x\in \Omega :\operatorname{dist} (x,\partial \Omega)>
\hat{\epsilon}\}\supseteq K
\]
and that, by Theorem~\ref{thm:2.25},
\begin{equation}\label{eq:3.52}
|\mu_\ell (\epsilon)-\mu_i|\leq 1
\end{equation}
for all $\ell =k_p+1,\dots , k_{p+1}$ and
$\epsilon \in (0,\hat{\epsilon}]$. Applying the parabolic Harnack
inequality, Proposition~\ref{prop:3.1}, with $\Sigma =\Omega$
or $\Sigma =\Omega (\epsilon)$
$(0<\epsilon \leq \frac{1}{2} \hat{\epsilon})$,
$\Sigma '=D$, $\omega =1$, $a_{ij}=\delta_{ij}$, $\tau _1=1$,
$\tau _2=2$, $t_1=5/4$, $\eta =\frac{1}{2}\hat{\epsilon}$ and
\begin{equation}\label{eq:3.53}
u(x,t)=e^{-\mu_it}\varphi_i (x)\quad (1<t<2,  x\in \Omega)
\end{equation}
or
\begin{equation} \label{eq:3.54}
u(x,t)=\big\| \sum^{k_{p+1}}_{\ell=k_p+1}a_{i,\ell }
(\epsilon )\varphi_\ell (\epsilon) \big\| ^{-1}_{L^2
(\Omega (\epsilon))} a_{i,q}(\epsilon)
e^{-\mu_q(\epsilon) t}\varphi_q (\epsilon)(x)
\end{equation}
for $x\in \Omega (\epsilon)$, $1<t<2$, $q=k_p+1$, $\dots $,
$k_{p+1}$ and $0<\epsilon \leq \frac{1}{2}\hat{\epsilon}$, where
\[
P_{\mathcal{H},\mathcal{B}(\epsilon)}\varphi_i
=1_{\Omega \cap \Omega(\epsilon)}\varphi_i
=\sum^\infty_{\ell=1} a_{i,\ell} (\epsilon) \varphi_\ell (\epsilon),
\]
we see that there exists $\alpha \in (0,1]$, depending only on $N$,
such that
\begin{equation}\label{eq:3.55}
|\varphi_i (x)-\varphi_i(y)|\leq A|x-y|^\alpha \quad
(x,y\in D)
\end{equation}
and, for  $\epsilon \in ( 0,\hat{\epsilon}/2)$,
\begin{equation}\label{eq:3.56}
|\psi _i (\epsilon)(x)-\psi_i(\epsilon )(y) |\leq A|x-y|^\alpha
\quad (x,y\in D),
\end{equation}
where (using \eqref{eq:3.52}),
\[
A=2(8/\hat{\epsilon})^\alpha (k_{p+1}-k_p)c(1)^{1/2}
e^{(\mu_i+1)/4} \max \{ e^{\lambda_q(B)/2}:k_p+1\leq q
\leq k_{p+1}\}.
\]
Note that the oscillation of
$ u(x,t)=e^{-\mu_it}\varphi_i(x)$
can be estimated using \eqref{eq:3.30} as follows:
\[
e^{-\mu_it}|\varphi_i (x)|\leq e^{-\mu_i}c(1)^{1/2}
e^{\lambda_i(B)/2}.
\]
Similarly the oscillation of
\[
u(x,t)=\big\| \sum^{k_{p+1}}_{\ell=k_p+1} a_{i,\ell}
(\epsilon)\varphi_\ell (\epsilon)\big\|^{-1}_{L
^2(\Omega (\epsilon))} a_{i,q}(\epsilon)
e^{-\mu_q (\epsilon )t} \varphi_q (\epsilon) (x)
\]
can be estimated by \eqref{eq:3.29} as follows:
\[
\big\| \sum^{k_{p+1}}_{\ell =k_p+1} a_{i,\ell} (\epsilon)
\varphi_\ell (\epsilon)\big\|^{-1}_{L^2(\Omega (\epsilon))}
a_{i,q} (\epsilon)e^{-\mu_q(\epsilon )t} \varphi_q(\epsilon )
\leq    e^{-\mu_q (\epsilon)} c(1)^{1/2} e^{\lambda_q(B)/2}.
\]
Let
$ r=\operatorname{dist} (K,\partial D)$ and
\[
\mathcal{R}=\min \{ r,\big( \frac{\delta}{6}\big)^{1/\alpha}
 A^{-\frac{1}{\alpha}}\}.
\]
Then for  $m=1,2,3,\dots$ and all $y\in D$ with
$|x_m-y|\leq \mathcal{R}$, by \eqref{eq:3.55} and \eqref{eq:3.56},
we have
\begin{gather}\label{eq:3.57}
|\varphi_i(x_m)-\varphi_i(y)|\leq \delta /6,\\
\label{eq:3.58} |\psi _i (\epsilon_m)(x_m)
-\psi_i (\epsilon_m)(y)|\leq \delta /6,
\end{gather}
and hence, by \eqref{eq:3.51}, \eqref{eq:3.57} and \eqref{eq:3.58},
\begin{equation}\begin{split}\label{eq:3.59}
|\varphi_i(y)-\psi_i(\epsilon _m)(y)|
&\geq |\varphi_i (x_m)-\psi_i(\epsilon_m)(x_m)|
 -|\varphi_i(x_m)-\varphi_i(y)|\\
&\quad -|\psi _i(\epsilon_m)(y) -\psi_i(\epsilon_m)(x_m)|\\
&\geq 2\delta /3.
\end{split}\end{equation}
Thus, for $m=1,2,3,\dots$, we have
\[
 \int_{B(x_m,R)} |\psi _i(\epsilon_m)(y)-\varphi_i (y)|^2\, dy
\geq c_2R^N\delta^2
\]
where $c_2>0$ depends only on $N$. But this contradicts
 \eqref{eq:2.89} of Theorem~\ref{thm:2.26}.
Therefore \eqref{eq:3.50} must hold and the theorem is proved.
\end{proof}

\section{Application to Koch snowflake}\label{sec:4}

In this section we let $\Omega \subseteq \mathbb{R}^2$ be the Koch
snowflake. Let $\{ \Omega _{\rm in}(n) \}^\infty_{n=1}$ be the usual
sequence of polygons approximating $\Omega$ from inside, with
$\Omega_{\rm in}(1)$ being an equilateral triangle. Let
$\{\Omega_{\rm out} (n)\}^\infty_{n=1}$ be the usual sequence  of
polygons approximating $\Omega$ from outside, with $\Omega_{\rm out}
(1)$ being a regular hexagon.

 We first recall the definition of $(\epsilon ,\delta)$-domains
(see \cite{J}):

\begin{definition}\label{def:4.1} \rm
Let $D$ be a domain in $\mathbb{R}^d$ and let $\epsilon >0$ and
$0<\delta\leq \infty$. We say that $D$ is an
$(\epsilon ,\delta)$-domain if for any two distinct points
$p_1$, $p_2\in D$ with $|p_1-p_2|\leq \delta$, there exists
a rectifiable path $\Gamma \subseteq D$ joining $p_1$ to $p_2$
satisfying the following conditions:
\begin{itemize}
\item[(i)] length $(\Gamma )\leq \epsilon^{-1} |p_1-p_2|$,
\item[(ii)] for all $p\in \Gamma$ we have
\begin{equation}\label{eq:4.1}
\operatorname{dist} (p,\partial D)\geq \epsilon |p_1-p_2|^{-1} |p-p_1||p-p_2|.
\end{equation}
\end{itemize}
We note that if $D$ is an $(\epsilon ,\delta)$-domain, then
any dilation of $D$ is also on $(\epsilon, \delta)$-domain.
\end{definition}

 We shall need the following result.

\begin{proposition}[{\cite[Proposition 3.2]{P2}}]\label{prop:4.2}
There exist $\hat{\epsilon}, \hat{\delta}>0$, independent of $n$,
such that $\Omega \times \mathbb{R}$ and
$\Omega_{\rm in}(n)\times \mathbb{R}$, $n=1,2,3,\dots $, are
 all $(\hat{\epsilon},\hat{\delta })$-domains in $\mathbb{R}^3$.
\end{proposition}

 Our main result in this section is as follows.


\begin{figure}[ht] 
\begin{center}
\setlength{\unitlength}{5mm}
\begin{picture}(18,14)(0,0)
\scriptsize
\drawline(0,5.196)(1,3.464)(3,3.464)(2,1.732)(3,0)(5,0)(6,1.73)(7,0)(9,0)(10,1.732)%
(9,3.464)(11,3.464)(12,5.196)(13,3.464)(15,3.464)(16,5.196)%
(15,6.938)(17,6.938)(18,8.66)(17,10.392)(15,10.392)(16,12.124)(15,13,856)%
(13,13.856)(12,12.124)(11,13.856)(9,13.856)(8,12,124)(9,10.392)(7,10.392)%
(6,8.66)(5,10.392)(3,10.392)(2,8.66)(3,6.938)(1,6.938)(0,5.196)
\dashline{0.2}(3,3.464)(5,3.464)(6,1.732)(7,3.364)(9,3.464)(8,5.196)(10,8.66)%
(9,10.392)(11,10.293)(12,12.124)(13,10.392)(15,10.392)(14,8.66)(15,6.938)%
(13,6.938)(12,5.196)(11,6.938)(7,6.938)(6,8.66)(5,6.938)(3,6.938)%
(4,5.196)(3,3.464)
\end{picture}
\end{center} 
\caption{The polygon $S$ in the proof of Theorem \ref{thm:4.3}} \label{fig1}
\end{figure}

\begin{theorem}\label{thm:4.3}
There exist $\check{\epsilon},\check{\delta} \in (0,\infty)$,
independent of $n$, such that $\Omega _{\rm out} (n)\times \mathbb{R}$
is an $(\check{\epsilon },\check{\delta})$-domain in $\mathbb{R}^3$
for all $n=1,2,3,\dots$.
\end{theorem}

\begin{proof}
Fix $n\in \mathbb{N}$ and let $(x_1, y_1, z_1)$,
$(x_2,y_2,z_2)\in \Omega_{\rm out} (n)\times \mathbb{R}$.
By Proposition~\ref{prop:4.2} we see that it suffices to consider
only the following two cases:
\begin{itemize}
\item[Case 1] Both $(x_1,y_1)$ and $(x_2,y_2)$ are in
$\Omega_{\rm out}(n)\backslash \Omega_{\rm in} (n+1)$,
\item[Case 2] $(x_1,y_1)\in \Omega_{\rm out}(n)\backslash
 \Omega _{\rm in} (n+1)$ but $(x_2,y_2)\in \Omega_{\rm in}(n+1)$.
\end{itemize}

 Let $S$ be the polygon in Figure~\ref{fig1}. Then, since $S\times \mathbb{R}$
is a Lipschitz domain, there exist $\tilde{\epsilon},\tilde{\delta }>0$
such that $S\times \mathbb{R}$ is an $(\tilde{\epsilon},
\tilde{\delta})$-domain in $\mathbb{R}^3$. Therefore,
since any dilation, translation, or rotation of $S\times \mathbb{R}$
is also an $(\tilde{\epsilon},\tilde{\delta})$-domain, we shall
assume that $(x_1,y_1)$ and $(x_2,y_2)$ are not both inside a domain
$R\subseteq \Omega _{\rm out} (n)$ that is obtained by a finite sequence
of dilations, translations, and rotations of $S$ and that some of
the edges of $R$ are also edges of $\Omega_{\rm out}(n)$.
This assumption implies that
 \begin{equation}\label{eq:4.2}
|(x_1,y_1)-(x_2,y_2)|\geq 3L_{\rm in}(n+1)
\end{equation}
 where $L_{\rm in}(n+1)$ denotes the length of each side of the polygon
$\Omega_{\rm in}(n+1)$. For every edge of $\Omega_{\rm out} (n)$
there corresponds two edges of $\Omega_{\rm in}(n+1)$ as shown in
 Figure~\ref{fig2}. 
 
\begin{figure}[ht] 
\begin{center}
\setlength{\unitlength}{1mm}
\begin{picture}(120,40)(0,0)
\scriptsize
\put(0,0){\line(3,4){30}}
\put(30,40){\line(3,-4){30}}
\put(60,0){\line(1,0){60}}
\dashline{1}(30,40)(120,0)
\dottedline{1}(30,40)(30,0)
\put(27,39){$v$}
\put(18,16.5){$a(x_1,y_1)$}
\put(29.3,19.4){$\bullet$}
\put(46,28){$\bullet$}
\put(46,25){$(x_1,y_1)$}
\qbezier(30,20)(40,20)(47,29)
\put(37,19){$\uparrow$}
\put(33,16){$\Gamma(x_1,y_1)$}
\end{picture}
\end{center} 
\caption{Edges: $--$ of $\Omega_{\rm out}(n)$ 
and --- of $\Omega_{\rm in}(n+1)$} \label{fig2}
\end{figure} 
 
 Referring to Figure~\ref{fig2}, suppose
$(x_1,y_1)\in \Omega_{\rm out}(n)\backslash \Omega_{\rm in}(n+1)$ and
suppose $(x_1,y_1)$ is within a distance of $\frac{1}{2} \cos
(\frac{\pi}{6}) L_{\rm in} (n+1) =\frac{\sqrt{3}}{4} L_{\rm
in}(n+1)$ from an acute vertex $v$ of $\Omega_{\rm in}(n+1)$. Then
we let $a(x_1,y_1)$ be the point on the angle bisector of
$\Omega_{\rm in}(n+1)$ at $v$ that is of the same distance from $v$ as
$(x_1,y_1)$ is from $v$. The arc of the circle, centered at $v$
and with radius $|v-(x_1,y_1)|$, starting at $a(x_1,y_1)$ and
ending at $(x_1,y_1)$ will be denoted by $\Gamma (x_1,y_1)$, see
Figure~\ref{fig2}. 

\begin{figure}[htb] 
\begin{center}
\setlength{\unitlength}{1mm}
\begin{picture}(120,40)(0,0)
\scriptsize
\put(0,0){\line(3,4){30}}
\put(30,40){\line(3,-4){30}}
\put(60,0){\line(1,0){60}}
\dashline{1}(30,40)(120,0)
\dottedline{1}(30,40)(30,0)
\put(27,39){$v$}
\put(-3,-1){$u$}
\put(56,-1){$w$}
\put(17,9.5){$a(x_1,y_1)$}
\put(29,12.4){$\bullet$}
\put(30,13){\line(1,0){31}}
\put(60,12.4){$\bullet$}
\put(59,9.5){$(x_1,y_1)$}
\put(35,9.5){$\Gamma(x_1,y_1)$}
\end{picture}
\end{center} 
\caption{Edges: $--$ of $\Omega_{\rm out}(n)$ 
and --- of $\Omega_{\rm in}(n+1)$}
\label{fig3}
\end{figure}

Referring to Figure~\ref{fig3}, suppose
$(x_1,y_1)\in \Omega_{\rm out}(n)\backslash \Omega_{\rm in}(n+1)$ and
suppose $(x_1,y_1)$ is not within a distance of  $\frac{1}{2} \cos
(\pi/6)L_{\rm in}(n+1)=\frac{\sqrt{3}}{4} L_{\rm in}(n+1)$ from any
acute vertex of $\Omega_{\rm in}(n+1)$. Then we let $a(x_1,y_1)$
be the center of the triangle with vertices $u$, $v$ and $w$. The
straight line segment joining $a(x_1,y_1)$ to $(x_1,y_1)$ will be
denoted by $\Gamma (x_1,y_1)$, see Figure~\ref{fig3}. Note that in
either case we have
\begin{equation}\label{eq:4.3}
\operatorname{length} (\Gamma (x_1,y_1))\leq 3L_{\rm in} (n+1).
\end{equation}
We shall assume that $n$ is sufficiently large so that
\begin{equation}\label{eq:4.4}
L_{\rm in}(n+1)\leq \hat{\delta}/9.
\end{equation}
Then if
\begin{equation}\label{eq:4.5}
|(x_1,y_1,z_1)-(x_2,y_2,z_2)|\leq \hat{\delta}/3,
\end{equation}
then, by \eqref{eq:4.3},
\begin{equation}\begin{split}\label{eq:4.6}
&|(a(x_1,y_1),z_1)-(a(x_2,y_2),z_2)|\\
&\leq   |(a(x_1,y_1),z_1)-(x_1,y_1,z_1)|
 +|(x_1,y_1,z_1)-(x_2,y_2,z_2)|\\
&\quad  +|(x_2,y_2,z_2)-(a(x_2,y_2),z_2)|\\
&\leq  \operatorname{length}(\Gamma (x_1,y_1))+\hat{\delta}/3
+\operatorname{length} (\Gamma (x_2,y_2))
\leq  \hat{\delta}.
\end{split}\end{equation}
We first present the proof for Case 1. We shall divide the proof
for this case into a number of subcases:


\subsection*{Case 1(i)}
 Here we assume that both $(x_1,y_1)$ and $(x_2,y_2)$ are in
$\Omega _{\rm out}(n)\backslash \Omega_{\rm in} (n+1)$,
that $(x_1,y_1)$ and $(x_2,y_2)$ are not both inside a region
$R\subseteq \Omega_{\rm out} (n)$ which is obtained from the polygon
$S$ in Figure~\ref{fig1} by a finite sequence of dilations and
isometries and that some of the edges of $R$ are also edges
of $\Omega_{\rm out} (n)$, that both $(x_1,y_1)$ and $(x_2,y_2)$
are within a distance of $\frac{1}{2}\cos (\pi/6)L_{\rm in}(n+1)
=\frac{\sqrt{3}}{4} L_{\rm in}(n+1)$ from some acute vertices
$v_1$ and $v_2$, respectively, of $\Omega_{\rm in}(n+1)$, and that
 \eqref{eq:4.4} and \eqref{eq:4.5} hold.

 Since $a(x_1,y_1)$, $a(x_2,y_2)\in \Omega_{\rm in}(n+1)$ and
\eqref{eq:4.5} holds, Proposition~\ref{prop:4.2} and \eqref{eq:4.6}
imply that there exists a rectifiable path
$\Gamma \subseteq \Omega_{\rm in}(n+1)\times \mathbb{R}$
joining $(a(x_1,y_1),z_1)$ to $(a(x_2,y_2),z_2)$ and satisfying:
\begin{itemize}
\item[(A)] $\operatorname{length}(\Gamma)\leq \hat{\epsilon}^{-1}|(a(x_1,y_1),z_1)-(a(x_2,y_2) ,z_2)|$
\item[(B)] for all $p\in \Gamma$ we have
\begin{equation} \label{eq:4.7}
\begin{split}
\operatorname{dist} (p,\partial \Omega_{\rm in}(n+1)\times \mathbb{R})
&\geq   \hat{\epsilon }\, |(a(x_1,y_1),z_1)-(a(x_2,y_2),z_2)|^{-1}\\
&\quad\times |p-(a(x_1,y_1),z_1)| |p-(a(x_2,y_2),z_2)|.
\end{split}\end{equation}
\end{itemize}

 Now, by \eqref{eq:4.2}, for $i=1,2$, we have
\begin{equation} \label{eq:4.8}
\operatorname{length} (\Gamma (x_i,y_i)) \leq \frac{\sqrt{3}}{4}
L_{\rm in}(n+1)\frac{\pi}{3}
\leq \frac{\sqrt{3}\pi}{36} |(x_1,y_1,z_1)-(x_2,y_2,z_2)|.
\end{equation}
Also we have, by (A) and \eqref{eq:4.8},
\begin{equation}\begin{split}\label{eq:4.9}
\operatorname{length} (\Gamma )
&\leq \hat{\epsilon}^{-1} |(a(x_1,y_1),z_1)-(a(x_2,y_2),z_2)|\\
&\leq \hat{\epsilon }^{-1} \big\{ |(a(x_1,y_1),z_1)-(x_1,y_1,z_1)|
 +|(x_1,y_1,z_1)-(x_2,y_2,z_2)|\\
&\quad +|(x_2,y_2,z_2)-(a(x_2,y_2),z_2)|\big\}\\
& \leq \hat{\epsilon}^{-1} \big( \frac{\sqrt{3}\pi}{18}  +1\big)
|(x_1,y_1,z_1)-(x_2,y_2,z_2)|.
\end{split}\end{equation}
In the reverse direction we have, by \eqref{eq:4.8},
\begin{equation}\begin{split}\label{eq:4.10}
&|(x_1,y_1,z_1)-(x_2,y_2,z_2)|\\
&\leq  |(x_1,y_1,z_1)-(a(x_1,y_1),z_1)|+|(a(x_1,y_1),z_1)-(a(x_2,y_2),z_2)|\\
&\quad +|(a(x_2,y_2),z_2)-(x_2,y_2,z_2)|\\
&\leq  \frac{\sqrt{3}\pi}{18} |(x_1,y_1,z_1)-(x_2,y_2,z_2)|
 +|(a(x_1,y_1),z_1)-(a(x_2,y_2) ,z_2)|
\end{split}\end{equation}
and hence
\begin{equation}\label{eq:4.11}
|(x_1,y_1,z_1)-(x_2,y_2,z_2)|\leq \big( 1-\frac{\sqrt{3}\pi}{18}
\big)^{-1} |(a(x_1,y_1),z_1)-(a(x_2,y_2),z_2)|.
\end{equation}
Let $p\in \Gamma$ and suppose that
\begin{equation}\label{eq:4.12}
|p-(a(x_i,y_i),z_i)|\geq \frac{1}{2}\operatorname{dist} (a(x_i,y_i),
\partial \Omega_{\rm in} (n+1))
\end{equation}
for $i=1,2$. Then, referring to Figure~\ref{fig2},
\begin{equation}\begin{split}\label{eq:4.13}
|p-(a(x_i,y_i),z_i)|&\geq \frac{1}{2}\sin \big(\frac{\pi}{6}\big)
 |a(x_i,y_i)-v_i|\\
&=\frac{3}{4\pi} |a(x_i,y_i)-v_i|\frac{\pi}{3}\\
&\geq \frac{3}{4\pi}|(a(x_i,y_i),z_i)-(x_i,y_i,z_i)|
\end{split}\end{equation}
for $i=1,2,$. Hence
\begin{equation}\begin{split}\label{eq:4.14}
|p-(x_i,y_i,z_i)|
&\leq |p-(a(x_i,y_i),z_i)|
 + |(a(x_i,y_i),z_i)-(x_i,y_i,z_i)|\\
&\leq \big( 1+\frac{4\pi}{3}\big) |p-(a(x_i,y_i),z_i)|
\end{split}\end{equation}
for $i=1,2$. Combining \eqref{eq:4.7}, \eqref{eq:4.9}
and \eqref{eq:4.14} we get
\begin{equation}\begin{split}\label{eq:4.15}
& \operatorname{dist} (p,\partial \Omega_{\rm out} (n)\times \mathbb{R})\\
&\geq   \operatorname{dist} (p,\partial \Omega_{\rm in} (n+1)\times \mathbb{R})\\
&\geq   \hat{\epsilon} \, |(a(x_1,y_1),z_1)-(a(x_2,y_2),z_2)|^{-1} |p-(a(x_1,y_1),z_1)|\\
&\quad \times |p-(a(x_2,y_2),z_2)|\\
&\geq  \hat{\epsilon } \big(\frac{\sqrt{3}\pi}{18} +1\big)^{-1}
\big( 1+\frac{4\pi}{3}\big)^{-2} |(x_1,y_1,z_1)-(x_2,y_2,z_2)|^{-1}\\
&\quad\times |p-(x_1,y_1,z_1)||p-(x_2,y_2,z_2)|.
\end{split}\end{equation}

 Next let $p\in \Gamma$ and suppose that
\begin{equation}\label{eq:4.16}
|p-(a(x_1,y_1),z_1)|<\frac{1}{2}\operatorname{dist} (a(x_1,y_1),\partial
\Omega_{\rm in} (n+1)).
\end{equation}
Referring to Figure~\ref{fig2}, we have, by \eqref{eq:4.16},
\begin{equation}\begin{split}\label{eq:4.17}
|p-(x_1,y_1,z_1)|&\leq |p-(a(x_1,y_1),z_1)|
 +|(a(x_1,y_1),z_1)-(x_1,y_1,z_1)|\\
&\leq \big(\frac{1}{4}+\frac{\pi}{3}\big)|a(x_1,y_1)-v_1|.
\end{split}\end{equation}
So, by \eqref{eq:4.16} and \eqref{eq:4.17},
\begin{equation}\begin{split} \label{eq:4.18}
 \operatorname{dist} (p,\partial \Omega_{\rm out} (n)\times \mathbb{R})
&\geq \operatorname{dist} (p,\partial \Omega_{\rm in}(n+1)\times \mathbb{R})\\
&\geq \frac{1}{2} \operatorname{dist} (a(x_1,y_1),\partial \Omega_{\rm in} (n+1))\\
&=\frac{1}{4} |a(x_1,y_1)-v_1|\\
&\geq \frac{1}{4} \big( \frac{1}{4} +\frac{\pi}{3}\big)^{-1}
 |p-(x_1,y_1,z_1)|.
\end{split}\end{equation}
Also, by \eqref{eq:4.16}, \eqref{eq:4.9}, \eqref{eq:4.8},
\eqref{eq:4.2},
\begin{equation}\begin{split}\label{eq:4.19}
&  |p-(x_2,y_2,z_2)|\\
&\leq |p-(a(x_1,y_1),z_1)|
 + |(a(x_1,y_1),z_1)-(a(x_2,y_2),z_2)|\\
&\quad +|(a(x_2,y_2),z_2)-(x_2,y_2,z_2)|\\
&\leq  \frac{1}{4} |a(x_1,y_1)-v_1|
+\big(\frac{\sqrt{3}\pi}{18} +1\big) |(x_1,y_1,z_1)-(x_2,y_2,z_2)|\\
&\quad +\frac{\sqrt{3}\pi}{36} |(x_1,y_1,z_1)-(x_2,y_2,z_2)|\\
&\leq  \frac{\sqrt{3}}{16} L_{\rm in}(n+1)
 +\big(\frac{\sqrt{3}\pi}{12} +1\big) |(x_1,y_1,z_1)-(x_2,y_2,z_2)|\\
&\leq  \frac{\sqrt{3}}{48} |(x_1,y_1)-(x_2,y_2)|
  + \big( \frac{\sqrt{3}\pi}{12} +1\big) |(x_1,y_1,z_1)-(x_2,y_2,z_2)|\\
&\leq  \big(\frac{\sqrt{3}}{48} +\frac{\sqrt{3}\pi}{12} +1\big)
|(x_1,y_1,z_1)-(x_2,y_2,z_2)|.
\end{split}\end{equation}
Combining \eqref{eq:4.18} and \eqref{eq:4.19} we obtain
\begin{equation}\begin{split}\label{eq:4.20}
&\operatorname{dist} (p,\partial \Omega_{\rm out} (n)\times \mathbb{R})\\
&\geq  \frac{1}{4} \big( \frac{1}{4} +\frac{\pi}{3}\big)^{-1}
\big( \frac{\sqrt{3}}{48} +\frac{\sqrt{3}\pi}{12} +1\big)^{-1} |(x_1,y_1,z_1)-(x_2,y_2,z_2)|^{-1}\\
&\quad \times |p-(x_1,y_1,z_1)||p-(x_2,y_2,z_2)|.
\end{split}\end{equation}
Now let $p=(x,y,z_1)\in \Gamma (x_1,y_1)\times \{z_1\}$ and let
\begin{equation}\label{eq:4.21}
k_1=\inf \{ b^{-1}\sin b:0<b<\frac{\pi}{3}\} >0.
\end{equation}



\begin{figure}[ht] 
\begin{center}
\setlength{\unitlength}{1mm}
\begin{picture}(120,40)(0,0)
\scriptsize
\put(0,0){\line(3,4){30}}
\put(30,40){\line(3,-4){30}}
\put(60,0){\line(1,0){60}}
\dashline{1}(30,40)(120,0)
\dottedline{1}(30,40)(30,0)
\put(26,40){$v_1$}
\put(18,16.5){$a(x_1,y_1)$}
\put(29.3,19.4){$\bullet$}
\put(46.7,28.6){$\bullet$}
\put(48,34){$(x_1,y_1)$}
\put(48.4,30.7){$\swarrow$}
\qbezier[20](30,20)(40,20)(47,29)
\put(44,25.9){$\bullet$}
\dottedline{1}(30,40)(75,0)
\dottedline{1}(30,40)(95,0)
\put(44.5,23){$(x,y)$}
\qbezier(61.5,12.2)(65,13)(66,18)
\put(65.5,12.5){$b$}
\qbezier(66,18)(69,19)(70,22)
\put(70,18){$a$}
\end{picture}
\end{center} 
\caption{Edges: $--$ of $\Omega_{\rm out}(n)$
and --- of $\Omega_{\rm in}(n+1)$} \label{fig4}
\end{figure}

Referring to Figure~\ref{fig4} we have
\begin{equation}\begin{split}\label{eq:4.22}
\operatorname{dist} (p, \partial \Omega_{\rm out} (n)\times \mathbb{R})
&=  \operatorname{dist} ((x,y),\partial \Omega_{\rm out} (n))\\
&=  |(x_1,y_1)-v_1|\sin (a+b)\\
&=  |(x_1,y_1)-v_1|b(b^{-1}\sin (a+b))\\
&\geq   |(x_1,y_1)-v_1|b(b^{-1}\sin b)\\
&\geq  |(x_1,y_1)-v_1|bk_1\\
&\geq  k_1 |(x_1,y_1)-(x,y)|\\
&=  k_1|(x_1,y_1,z_1)-(x,y,z_1)|.
\end{split}\end{equation}
Also we have, for $p=(x,y,z_1) \in \Gamma (x_1,y_1)\times \{ z_1\}$,
\begin{equation}\begin{split}\label{eq:4.23}
|p-(x_2,y_2,z_2)|
&\leq  |p-(x_1,y_1,z_1)|+|(x_1,y_1,z_1)-(x_2,y_2,z_2)|\\
&\leq  \frac{\pi\sqrt{3}}{12} L_{\rm in} (n+1)+|(x_1,y_1,z_1)-(x_2,y_2,z_2)|\\
&\leq  \big( \frac{\pi \sqrt{3}}{36} +1\big)
|(x_1,y_1,z_1)- (x_2,y_2,z_2)|
\end{split}\end{equation}
where we have used \eqref{eq:4.2}. Thus, combining \eqref{eq:4.22}
and \eqref{eq:4.23}, we have, for all
$p=(x,y,z_1)\in \Gamma (x_1,y_1)\times \{z_1\}$,
\begin{equation}\begin{split}\label{eq:4.24}
\operatorname{dist} (p,\partial \Omega_{\rm out} (n)\times \mathbb{R})
&\geq  \Big( \frac{\pi\sqrt{3}}{36} +1\Big)^{-1}
 k_1 |(x_1,y_1,z_1)-(x_2,y_2,z_1)|^{-1}\\
&\quad\times |p-(x_1,y_1,z_1)||p-(x_2,y_2,z_2)|.
\end{split}\end{equation}
Similarly, we have, for all
$p=(x,y,z_2)\in \Gamma (x_2,y_2)\times \{ z_2\}$,
\begin{equation}\begin{split}\label{eq:4.25}
\operatorname{dist} (p,\partial \Omega_{\rm out} (n)\times \mathbb{R})
&\geq  \Big( \frac{\pi \sqrt{3}}{36} +1\Big)^{-1}
 k_1 |(x_1,y_1,z_1)-(x_2,y_2,z_2)|\\
&\quad\times |p-(x_1,y_1,z_1)||p-(x_2,y_2,z_2)|.
\end{split}\end{equation}
From \eqref{eq:4.5}, \eqref{eq:4.6}, \eqref{eq:4.8}, \eqref{eq:4.9}, \eqref{eq:4.15}, 
\eqref{eq:4.20}, \eqref{eq:4.24} and \eqref{eq:4.25}, we see that 
if $(x_1, y_1, z_1)$ and $(x_2,y_2,z_2)$ satisfy the assumptions of Case 1(i) and if
\begin{equation}\label{eq:4.26}
|(x_1,y_1,z_1)-(x_2,y_2,z_2)|\leq \hat{\delta}/3,
\end{equation}
then there exists a path
\begin{equation}\label{eq:4.27}
 \tilde{\Gamma} =(\Gamma (x_1,y_1)\times \{ z_1\})+\Gamma
+(\Gamma (x_2,y_2)\times \{z_2\})
\end{equation}
joining $(x_1,y_1,z_1)$ to $(x_2,y_2,z_2)$ satisfying
\begin{equation}\label{eq:4.28}
\operatorname{length}(\tilde{\Gamma}) \leq \big[ \frac{\sqrt{3}\pi}{18}
+\hat{\epsilon } \big( \frac{\sqrt{3}\pi}{18} +1\big)\big]
 |(x_1,y_1,z_1)-(x_2,y_2,z_2)|
\end{equation}
and for all $p\in \tilde{\Gamma}$ we have
\begin{equation}\begin{split}\label{eq:4.29}
&\operatorname{dist}(p,\partial \Omega_{\rm out}(n)\times \mathbb{R})\\
&\geq  \epsilon_1 |(x_1,y_1,z_1)-(x_2,y_2,z_2)|^{-1}|p
-(x_1,y_1,z_1)||p-(x_2,y_2,z_2)|
\end{split}\end{equation}
where
\begin{equation}\begin{split}\label{eq:4.30}
\epsilon_1 &= \min \Big\{ \hat{\epsilon}
\Big( \frac{\sqrt{3}\pi}{18} +1\Big)^{-1}
  \Big( 1+\frac{4\pi}{3}\Big)^{-2},\\
&\quad \frac{1}{4} \Big( \frac{1}{4} +\frac{\pi}{3}\Big)^{-1}
 \Big( \frac{\sqrt{3}}{48} +\frac{\sqrt{3}\pi}{12}+1\Big)^{-1},
 k_1 \Big( \frac{\sqrt{3}\pi}{36} +1\Big)^{-1} \Big\}.
\end{split}\end{equation}


\subsection*{Case 1(ii)}
 Here we assume that both $(x_1,y_1)$ and $(x_2,y_2)$ are in
$\Omega _{\rm out} (n)\backslash \Omega_{\rm in} (n+1)$, that $(x_1,y_1)$
and $(x_2,y_2)$ are not both inside a region
$R\subseteq \Omega_{\rm out} (n)$ which is obtained from the polygon
$S$ in Figure~\ref{fig1} by a finite sequence of dilations and
isometries and that some of the edges of $R$ are also edges of
$\Omega _{\rm out }(n)$, that both $(x_1,y_1)$ and $(x_2,y_2)$
are not within a distance of
$\frac{1}{2}\cos (\pi /6) L_{\rm in} (n+1)
=\frac{\sqrt{3}}{4} L_{\rm in} (n+1)$
from any acute vertex of $\Omega_{\rm in}(n+1)$, and that \eqref{eq:4.4}
and \eqref{eq:4.5} hold.


\begin{figure}[ht]
\begin{center}
\setlength{\unitlength}{1mm}
\begin{picture}(120,50)(0,-10)
\scriptsize
\put(0,0){\line(3,4){30}}
\put(30,40){\line(3,-4){30}}
\put(60,0){\line(1,0){60}}
\dashline{1}(30,40)(120,0)
\put(120,0){\line(-3,-4){10}}
\dottedline{1}(30,40)(30,0)
\put(29.4,39){$\bullet$}
\put(26.8,39){$v$}
\put(29,39){$\bullet$}
\put(-1,-1){$\bullet$}
\put(-3,-1){$u$}
\put(59.4,-.8){$\bullet$}
\put(56.5,-1){$w$}
\put(119,-.8){$\bullet$}
\put(121,-1){$\sigma$}
\dottedline{1}(30,13)(40,35)
\dottedline{1}(30,13)(50.5,30)
\put(50.4,29.9){$\bullet$}
\put(52,32){$\alpha$}
\qbezier[20](30,13)(47,15)(50.6,30)
\dottedline{1}(30,13)(61.6,3)
\put(55.8,4){$\bullet$}
\put(53.5,3){$\tau$}
\put(60.8,2.4){$\bullet$}
\put(63.5,2){$\eta$}
\dottedline{1}(54,13)(60,26)
\qbezier(56.6,13)(56.6,14.8)(55,15.5)
\put(57,14.2){$\theta$}
\dottedline{1}(60,0)(70,22)
\put(69.5,21.3){$\bullet$}
\put(71.5,23){$\gamma$}
\put(30,13){\line(1,0){31}}
\put(29,12.3){$\bullet$}
\put(19,10){$a(x_1,y_1)$}
\put(60,12.3){$\bullet$}
\put(55,10){$(x_1,y_1)$}
\qbezier(35,11.5)(36.3,16)(32.5,18)
\put(36.5,14.5){$\beta_2$}
\qbezier(37,18.5)(36,20.2)(33.6,21.5)
\put(36.5,21.5){$\beta_1$}
\end{picture}
\end{center}
\caption{Edges: $--$ of $\Omega_{\rm out}(n)$ and
--- of $\Omega_{\rm in}(n+1)$} \label{fig5}
\end{figure}

 In Figure~\ref{fig5}, let $\theta$ be the angle between
the line segment $\overline{(x_1,y_1),a(x_1,y_1)}$ joining
$(x_1,y_1)$ to $a(x_1,y_1)$ and the line perpendicular to the
line segment $\overline{v,\sigma}$ joining $v$ to $\sigma$.
Let $\alpha$ be the point on $\overline{v,\sigma}$ such that the
length of $\overline{v,\alpha}$ is $\frac{1}{2}\cos (\pi/6)L_{\rm in}(n+1)$. Let $\gamma $ be the midpoint of $\overline{v,\sigma}$ and let $\eta $ be a point on $\overline{\gamma, w}$ such that
\begin{equation}\label{eq:4.31}
\operatorname{length}(\overline{\gamma ,\eta})
=\frac{3}{4}\operatorname{length}(\overline{\gamma, w}).
\end{equation}
Let $\beta_1$ and $\beta_2$ be the angles between the line
perpendicular to $\overline{v,\sigma}$ and the line segments
$\overline{a(x_1,y_1),\alpha}$ and $\overline{a(x_1,y_1),\eta}$,
respectively. Let $\tau$ be the point of intersection of the
line segments $\overline{v,w}$ and $\overline{a(x_1,y_1),\eta}$. If
\begin{equation}\label{eq:4.32}
\beta _1\leq \theta \leq \beta_2,
\end{equation}
then, for all $(x,y)\in \overline{a(x_1,y_1),(x_1,y_1)}$, we have
\begin{equation}\label{eq:4.33}
 \operatorname{dist} ((x,y),\partial \Omega_{\rm out}(n))
\geq (\cos \theta) |(x,y)-(x_1,y_1)|
\geq (\cos \beta_1)|(x,y)-(x_1,y_1)|.
\end{equation}
If
\begin{equation}\label{eq:4.34}
\beta_2 < \theta < \frac{\pi}{2};
\end{equation}
i.e., if $(x_1,y_1)\in \Delta (\tau, \eta ,w)$, where
$\Delta (\tau ,\eta ,w)$ denotes the triangle with vertices
$\tau$, $\eta$ and $w$, then, for all
$(x,y)\in\overline{a(x_1,y_1),(x_1,y_1)}$, we have
\begin{equation}\begin{split}\label{eq:4.35}
\operatorname{dist} ((x,y) ,\partial \Omega _{\rm out} (n))
&\geq  \operatorname{dist} (\Delta (a(x_1,y_1),\eta ,w),\partial \Omega_{\rm out} (n))\\
&=   |\eta -\gamma |\\
&=  3 |\eta -w|\\
&=  k_2 |a(x_1,y_1)-\eta | \\
&\geq   k_2 |(x,y)-(x_1,y_1)|
\end{split}
\end{equation}
for some $k_2>0$ independent of $n$, $(x_1,y_1)$ and $(x_2,y_2)$.

  Combining \eqref{eq:4.33} and \eqref{eq:4.35} we have, for all $p=(x,y,z_1)\in \Gamma (x_1,y_1)\times \{ z_1\}$,
\begin{equation}\label{eq:4.36}
\operatorname{dist} (p,\partial \Omega _{\rm out} (n)\times \mathbb{R})
\geq  \min \{ \cos \beta_1,k_2 \} |p-(x_1,y_1,z_1)|.
\end{equation}
Also, by \eqref{eq:4.2}, for all
$p=(x,y,z_1)\in \Gamma (x_1,y_1)\times \{z_1\}$, we have
\begin{equation}\begin{split}\label{eq:4.37}
 |p-(x_2,y_2,z_2)|
&\leq  |p-(x_1,y_1,z_1)|+|(x_1,y_1,z_1)-(x_2,y_2,z_2)|\\
&\leq  L_{\rm in} (n+1) +|(x_1,y_1,z_1)-(x_2,y_2,z_2)|\\
&\leq  \frac{4}{3}
|(x_1,y_1,z_1)-(x_2,y_2,z_2)|.
\end{split}\end{equation} Thus
combining \eqref{eq:4.36} and \eqref{eq:4.37} we have, for all
$p=(x,y,z_1)\in \Gamma (x_1,y_1)\times \{z_1\}$,
\begin{equation}\begin{split}\label{eq:4.38}
\operatorname{dist} (p,\partial \Omega_{\rm out} (n)\times \mathbb{R})
&\geq  \frac{3}{4} \min \{\cos \beta_1 ,k_2\} |(x_1,y_1,z_1)-(x_2,y_2,z_2)|^{-1}\\
&\quad \times |p-(x_1,y_1,z_1)| |p-(x_2,y_2,z_2)|.
\end{split}\end{equation}
Similarly, for all $p=(x,y,z_2)\in\Gamma (x_2,y_2)\times \{ z_2\}$,
we have
\begin{equation}\begin{split}\label{eq:4.39}
\operatorname{dist} (p,\partial \Omega_{\rm out} (n)\times \mathbb{R})
&\geq  \frac{3}{4} \min \{\cos \beta_1,k_2\} |(x_1,y_1,z_1)-(x_2,y_2,z_2)|^{-1}\\
& \quad \times |p-(x_1,y_1,z_1) | |p-(x_2,y_2,z_2)|.
\end{split}\end{equation}
Referring to Figure~\ref{fig5} we have, by \eqref{eq:4.2},
\begin{equation}\begin{split}\label{eq:4.40}
\operatorname{length}(\Gamma (x_1,y_1)\times \{ z_1\})
&=\operatorname{length}(\Gamma (x_1,y_1))\\
&\leq L_{\rm in} (n+1)\\
&\leq \frac{1}{3}|(x_1,y_1,z_1)-(x_2,y_2,z_2)|.
\end{split}\end{equation}
Similarly we have
\begin{equation}\label{eq:4.41}
\operatorname{length}(\Gamma (x_2,y_2)\times \{ z_2\})
\leq \frac{1}{3} |(x_1,y_1,z_1)-(x_2,y_2,z_2)|.
\end{equation}
So, from \eqref{eq:4.39} and \eqref{eq:4.40}, we have
\begin{equation}\begin{split}\label{eq:4.42}
\operatorname{length}(\Gamma )
&\leq \hat{\epsilon}^{-1} |(a(x_1,y_1),z_1)-(a(x_2,y_2),z_2)|\\
&\leq \hat{\epsilon }^{-1} \{ |(a(x_1,y_1),z_1)-(x_1,y_1,z_1)|+|(x_1,y_1,z_1)-(x_2,y_2,z_2)|\\
&\quad + |(x_2,y_2,z_2)-(a(x_2,y_2),z_2)|\\
&\leq \frac{5}{3} \hat{\epsilon}^{-1} |(x_1,y_1,z_1)-(x_2,y_2,z_2)|.
\end{split}\end{equation}
Now let $p\in \Gamma$ and suppose that
\begin{equation}\label{eq:4.43}
 |p-(a(x_i,y_i),z_i)|\geq \frac{1}{2}\operatorname{dist} (a(x_i,y_i),
\partial \Omega_{\rm in} (n+1))
\end{equation}
for $i=1,2$. Then, referring to Figure~\ref{fig3}, we have
\begin{equation}\label{eq:4.44}
|p-(a(x_i,y_i),z_i)|\geq \frac{1}{4\sqrt{3}} L_{\rm in} (n+1)
\geq \frac{1}{4\sqrt{3}} |(a(x_i,y_i),z_i)-(x_i,y_i,z_i)|
\end{equation}
for $i=1,2$. Hence
\begin{equation}\begin{split}\label{eq:4.45}
 |p-(x_i,y_i,z_i)|&\leq |p-(a(x_i,y_i),z_i)|
 + |(a(x_i,y_i),z_i)-(x_i,y_i,z_i)|\\
& \leq (1+4\sqrt{3})|p-(a(x_i,y_i),z_i)|
\end{split}\end{equation}
for $i=1,2$. Thus, by \eqref{eq:4.42},
\begin{equation}\begin{split}\label{eq:4.46}
\operatorname{dist} (p,\partial \Omega_{\rm out}(n)\times \mathbb{R})
&\geq   \operatorname{dist} (p,\partial \Omega_{\rm in} (n+1)\times \mathbb{R})\\
&\geq   \hat{\epsilon} |(a(x_1,y_1),z_1)-(a(x_2,y_2),z_2)|^{-1}\\
&\times |p-(a(x_1,y_1),z_1)||p-(a(x_2,y_2),z_2)|\\
&\geq   \frac{3}{5} (1+4\sqrt{3})^{-2} \hat{\epsilon} |(x_1,y_1,z_1)-(x_2,y_2,z_2)|^{-1}\\
&\quad \times |p-(x_1,y_1,z_1)| |p-(x_2,y_2,z_2)|.
\end{split}\end{equation}
Next let $p\in \Gamma$
and suppose that
\[
|p-(a(x_1,y_1),z_1) |<\frac{1}{2} \operatorname{dist} (a(x_1,y_1),
\partial \Omega_{\rm in}(n+1)).
\]
Then, referring to Figure~\ref{fig3},
\begin{equation}\begin{split}\label{eq:4.47}
\operatorname{dist} (p,\partial \Omega_{\rm out} (n)\times \mathbb{R})
&\geq  \operatorname{dist} (p,\partial \Omega_{\rm in} (n+1)\times \mathbb{R})\\
&\geq  \frac{1}{2}\operatorname{dist} ((a(x_1,y_1),z_1),\partial \Omega_{\rm in} (n+1)\times \mathbb{R})\\
&=  \frac{1}{4\sqrt{3}} L_{\rm in} (n+1)
\end{split}\end{equation}
and
\begin{equation}\begin{split}\label{eq:4.48}
|p-(x_1,y_1,z_1)|&\leq |p-(a(x_1,y_1),z_1)|+|(a(x_1,y_1),z_1)
 -(x_1,y_1,z_1)|\\
&\leq \frac{1}{2} \operatorname{dist} (a(x_1,y_1),\partial \Omega_{\rm in} (n+1))+L_{\rm in} (n+1)\\
&= \big(\frac{1}{4\sqrt{3}}+1\big) L_{\rm in} (n+1),
\end{split}\end{equation}
hence, from \eqref{eq:4.47} and \eqref{eq:4.48},
\begin{equation}\label{eq:4.49}
\operatorname{dist} (p,\partial \Omega_{\rm out} (n)\times \mathbb{R})\geq
\frac{1}{4\sqrt{3}} \big( \frac{1}{4\sqrt{3}}+1\big)^{-1}
|p-(x_1,y_1,z_1)|.
\end{equation}
Also, by \eqref{eq:4.48} and \eqref{eq:4.2}, we have
\begin{equation}\begin{split}\label{eq:4.50}
|p-(x_2,y_2,z_2)| &\leq |p-(x_1,y_1,z_1)|+|(x_1,y_1,z_1)-(x_2,y_2,z_2)|\\
&\leq \big[ \big(\frac{1}{4\sqrt{3}} +1\big) 3^{-1} +1\big]
|(x_1,y_1,z_1)-(x_2,y_2,z_2)|.
\end{split}\end{equation}
Combining \eqref{eq:4.49} and \eqref{eq:4.50} we obtain
\begin{equation}\begin{split}\label{eq:4.51}
&\operatorname{dist} (p,\partial \Omega_{\rm out} (n)\times \mathbb{R})\\
&\geq  \frac{1}{4\sqrt{3}} \Big( \frac{1}{4\sqrt{3}} +1\Big) ^{-1}
 \Big[ \big( \frac{1}{4\sqrt{3}}+1\big) 3^{-1} +1\Big]^{-1}
|(x_1,y_1,z_1) -(x_2,y_2,z_2)|^{-1}\\
&\quad  \times |p-(x_1,y_1,z_1)||p-(x_2,y_2,z_2)|.
\end{split}\end{equation}
By symmetry, if $p\in \Gamma$ and if
\[
|p-(a(x_2,y_2),z_2)|<\frac{1}{2}\operatorname{dist} (a(x_2,y_2),
\partial \Omega_{\rm in} (n+1)),
\]
then we have
\begin{equation}\begin{split}\label{eq:4.52}
&\operatorname{dist} (p,\partial \Omega_{\rm out} (n)\times \mathbb{R})\\
&\geq  \frac{1}{4\sqrt{3}} \left( \frac{1}{4\sqrt{3}} +1\right)^{-1} \left[ \left( \frac{1}{4\sqrt{3}}+1\right) 3^{-1} +1\right]^{-1} |(x_1,y_1,z_1)-(x_2,y_2,z_2)|^{-1}\\
&\quad \times |p-(x_1,y_1,z_1)||p-(x_2,y_2,z_2)|.
\end{split}\end{equation}
Thus from \eqref{eq:4.5}, \eqref{eq:4.6}, \eqref{eq:4.38},
\eqref{eq:4.39}, \eqref{eq:4.40}, \eqref{eq:4.41}, \eqref{eq:4.42},
\eqref{eq:4.46}, \eqref{eq:4.51} and \eqref{eq:4.52},
we see that if $(x_1,y_1,z_1)$ and $(x_2,y_2,z_2)$ satisfy the
assumptions of Case~1(ii) and if
\[
|(x_1,y_1,z_1)-(x_2,y_2,z_2)|\leq \hat{\delta}/3,
\]
then there exists a path
\begin{equation}\label{eq:4.53}
\tilde{\Gamma} =(\Gamma (x_1,y_1)\times \{ z_1\})+\Gamma
+(\Gamma (x_2,y_2)\times \{ z_2\})
\end{equation}
joining $(x_1,y_1,z_1)$ to $(x_2,y_2,z_2)$ satisfying
\begin{equation}\label{eq:4.54}
\operatorname{length}(\tilde{\Gamma})\leq
\big( \frac{2}{3} +\frac{5}{3} \hat{\epsilon}^{-1} \big)
|(x_1,y_1,z_1)-(x_2,y_2,z_2)|
\end{equation}
and for all $p\in \tilde{\Gamma}$ we have
\begin{equation}\begin{split}\label{eq:4.55}
&  \operatorname{dist} (p,\partial \Omega_{\rm out} (n)\times \mathbb{R})\\
&\geq  \epsilon_2 |(x_1,y_1,z_1)-(x_2,y_2,z_2)|^{-1} |p
-(x_1,y_1,z_1) | |p-(x_2,y_2,z_2)|
\end{split}\end{equation}
where
\begin{equation}\begin{split}\label{eq:4.56}
\epsilon_2 &=\min \Big\{ \frac{3}{4}\cos \beta_1 ,  \frac{3}{4} k_2,
 \frac{3}{5} (1+4\sqrt{3})^{-2} \hat{\epsilon},\\
&\quad  \frac{1}{4\sqrt{3}} \Big( \frac{1}{4\sqrt{3}} +1\Big)^{-1}
 \Big[ \big( \frac{1}{4\sqrt{3}} +1\big) 3^{-1} +1\Big]^{-1}\Big\}.
\end{split}\end{equation}

\subsection*{Case 1(iii)}
 Here we assume that both $(x_1,y_1)$ and $(x_2,y_2)$ are in
$\Omega_{\rm out} (n)\backslash \Omega_{\rm in} (n+1)$, that $(x_1,y_1)$
 and $(x_2,y_2)$ are not both inside a region
$R\subseteq \Omega_{\rm out} (n)$ which is obtained from the polygon
$S$ in Figure~\ref{fig1} by a finite sequence of dilations and
isometries and that some of the edges of $R$ are also edges of
$\Omega_{\rm out} (n)$, that $(x_1,y_1)$ is not within a distance of
$\frac{1}{2}\cos (\pi/6)L_{\rm in} (n+1)$ from any acute vertex of
$\Omega_{\rm in} (n+1)$, that $(x_2,y_2)$ is within a distance
of $\frac{1}{2} \cos (\pi/6)L_{\rm in} (n+1)$ from an acute vertex
$v_2$ of $\Omega_{\rm in} (n+1)$, and that \eqref{eq:4.4} and
\eqref{eq:4.5} hold.

 In this case, by \eqref{eq:4.2}, we have
\begin{equation}\begin{split}\label{eq:4.57}
\operatorname{length}(\Gamma (x_2,y_2)\times \{ z_1\})
&\leq \frac{\pi}{3} |(x_2,y_2,z_2)-v_2|\\
&\leq \frac{\pi \sqrt{3}}{12} L_{\rm in} (n+1)\\
&\leq \frac{\pi\sqrt{3}}{36} |(x_1,y_1,z_1)-(x_2,y_2,z_2)|
\end{split}\end{equation}
and, referring to Figure~\ref{fig5},
\begin{equation}\begin{split}\label{eq:4.58}
\operatorname{length}(\Gamma (x_1,y_1)\times \{ z_1\})
&= |a(x_1,y_1)-(x_1,y_1)|\\
&\leq L_{\rm in} (n+1)\\
&\leq \frac{1}{3} |(x_1,y_1,z_1)-(x_2,y_2,z_2)|.
\end{split}\end{equation}
Hence
\begin{equation}\begin{split}\label{eq:4.59}
\operatorname{length}(\Gamma )
&\leq  \hat{\epsilon}^{-1} |(a(x_1,y_1),z_1) -(a(x_2,y_2),z_2)|\\
&\leq  \hat{\epsilon}^{-1} \{ | (a(x_1,y_1),z_1) -(x_1,y_1,z_1)|
 + |(x_1,y_1,z_1)-(x_2,y_2,z_2)|\\
&\quad + |(x_2,y_2,z_2)-(a(x_2,y_2),z_2)|\}\\
&\leq  \hat{\epsilon}^{-1} \big( \frac{4}{3}
+\frac{\pi\sqrt{3}}{36} \big) |(x_1,y_1,z_1) -(x_2,y_2,z_2)|.
\end{split}\end{equation}
From \eqref{eq:4.57} and \eqref{eq:4.58} we  have
\begin{align*}
&|(x_1,y_1,z_1)-(x_2,y_2,z_2)|\\
&\leq  |(x_1,y_1,z_1)-(a(x_1,y_1),z_1)|+|(a(x_1,y_1),z_1)
 -(a(x_2,y_2),z_2)|\\
&\quad + |(a(x_2,y_2),z_2)-(x_2,y_2,z_2)|\\
&\leq  \frac{1}{3} |(x_1,y_1,z_1)-(x_2,y_2,z_2)|
 + |(a(x_1,y_1),z_1)-(a(x_2,y_2),z_2)|\\
&\quad + \frac{\pi \sqrt{3}}{36} |(x_1,y_1,z_1)-(x_2,y_2,z_2)|,
\end{align*}
hence
\begin{equation}\label{eq:4.60}
|(x_1,y_1,z_1)-(x_2,y_2,z_2)|
\leq  \Big( \frac{2}{3}-\frac{\pi\sqrt{3}}{36} \Big)^{-1}
|(a(x_1,y_1),z_1)-(a(x_2,y_2),z_2)|.
\end{equation}
Let $p\in \Gamma$ and suppose that
\[
|p-(a(x_i,y_i),z_i)|\geq \frac{1}{2} \operatorname{dist} (a(x_i,y_i),
\partial \Omega _{\rm in} (n+1))
\]
for $i=1,2$. Then
\[
 |p-(a(x_1,y_1),z_1)|\geq \frac{1}{4\sqrt{3}} L_{\rm in} (n+1)
\geq \frac{1}{4\sqrt{3}} |(a(x_1,y_1),z_1)-(x_1,y_1,z_1)|
\]
and so
\begin{equation}\begin{split}\label{eq:4.61}
|p-(x_1,y_1,z_1)|&\leq |p-(a(x_1,y_1),z_1)|
 +|(a(x_1,y_1),z_1)-(x_1,y_1,z_1)|\\
&\leq (1+4\sqrt{3})|p-(a(x_1,y_1),z_1)|.
\end{split}\end{equation}
Also
\begin{align*}
|p-(a(x_2,y_2),z_2)|&\geq \frac{1}{2}\sin (\pi/6) |a(x_2,y_2)-v_2|\\
&=\frac{3}{4\pi} |a(x_2,y_2)-v_2|\frac{\pi}{3}\\
&\geq \frac{3}{4\pi} |(a(x_2,y_2),z_2)-(x_2,y_2,z_2)|,
\end{align*}
and hence
\begin{equation}\begin{split}\label{eq:4.62}
|p-(x_2,y_2,z_2)|&\leq |p-(a(x_2,y_2),z_2)|
 + |(a(x_2,y_2),z_2)-(x_2,y_2,z_2)|\\
&\leq \big( 1+\frac{4\pi}{3} \big) |p-(a(x_2,y_2),z_2)|.
\end{split}\end{equation}
Thus, by \eqref{eq:4.59}, \eqref{eq:4.61} and \eqref{eq:4.62},
\begin{equation}\begin{split} \label{eq:4.63}
&\operatorname{dist} (p,\partial \Omega_{\rm out} (n)\times \mathbb{R})\\
&\geq  \operatorname{dist} (p,\partial \Omega_{\rm in} (n+1)\times \mathbb{R})\\
&\geq  \hat{\epsilon} |(a(x_1,y_1),z_1)-(a(x_2,y_2),z_2)|^{-1}
 |p-(a(x_1,y_1),z_1)|\\
&\quad\times |p-(a(x_2,y_2),z_2)|\\
&\geq  \hat{\epsilon} \big( \frac{4}{3}+\frac{\pi\sqrt{3}}{36}
 \big)^{-1} (1+4\sqrt{3} )^{-1} \Big( 1+\frac{4\pi}{3}\Big)^{-1}\\
&\quad \times |(x_1,y_1,z_1)-(x_2,y_2,z_2)|^{-1} |p-(x_1,y_1,z_1)|
 |p-(x_2,y_2,z_2)|.
\end{split}\end{equation}
Next let $p\in \Gamma$ and suppose that
\[
|p-(a(x_1,y_1),z_1)|<\frac{1}{2}\operatorname{dist} (a(x_1,y_1),
\partial\Omega_{\rm in} (n+1)).
\]
Then \eqref{eq:4.47}, \eqref{eq:4.48}, \eqref{eq:4.49} and
\eqref{eq:4.50} still hold. Hence we have
\begin{equation}\begin{split}\label{eq:4.64}
&\operatorname{dist} (p,\partial \Omega_{\rm out} (n)\times \mathbb{R})\\
&\geq  \frac{1}{4\sqrt{3}} \Big( \frac{1}{4\sqrt{3}}+1\Big)^{-1}
\Big[ \big( \frac{1}{4\sqrt{3}} +1\big) 3^{-1} +1\Big]^{-1}\\
&\quad\times |(x_1,y_1,z_1)-(x_2,y_2,z_2)|^{-1} |p-(x_1,y_1,z_1)|
 |p-(x_2,y_2,z_2)|.
\end{split}\end{equation}
Now let $p\in \Gamma$ and suppose that
\[
|p-(a(x_2,y_2),z_2)|<\frac{1}{2}\operatorname{dist} (a(x_2,y_2),
\partial \Omega_{\rm in}(n+1)).
\]
Then
\begin{equation}\begin{split}\label{eq:4.65}
|p-(x_2,y_2,z_2)|&\leq |p-(a(x_2,y_2),z_2)|
 + |(a(x_2,y_2),z_2)-(x_2,y_2,z_2)|\\
&\leq \big( \frac{1}{4} +\frac{\pi}{3}\big) |a(x_2,y_2)-v_2|.
\end{split}\end{equation}
So
\begin{equation}\begin{split}\label{eq:4.66}
\operatorname{dist} (p,\partial \Omega_{\rm out} (n)\times \mathbb{R})
&\geq  \operatorname{dist} (p,\partial \Omega_{\rm in} (n+1)\times \mathbb{R})\\
&\geq  \frac{1}{2} \operatorname{dist} (a(x_2,y_2),\partial \Omega_{\rm in} (n+1))\\
&=  \frac{1}{4} |a(x_2,y_2)-v_2|\\
&\geq  \frac{1}{4} \Big( \frac{1}{4}+\frac{\pi}{3}\Big)^{-1}
|p-(x_2,y_2,z_2)|.
\end{split}\end{equation}
Also we have, by \eqref{eq:4.59}, \eqref{eq:4.58} and \eqref{eq:4.2},
\begin{align} 
 |p-(x_1,y_1,z_1)|
&\leq  |p-(a(x_2,y_2),z_2)|+|(a(x_2,y_2),z_2)-(a(x_1,y_1),z_1)| \nonumber\\
&\quad + |(a(x_1,y_1),z_1)-(x_1,y_1,z_1)| \nonumber \\
&\leq  \frac{1}{4} |a(x_2,y_2)-v_2|
 +\big( \frac{4}{3} +\frac{\pi\sqrt{3}}{36} \big) |(x_1,y_1,z_1)-(x_2,y_2,z_2)|
  \nonumber\\
&\quad +\frac{1}{3} |(x_1,y_1,z_1)-(x_2,y_2,z_2)| \label{eq:4.67} \\
&\leq  \frac{\sqrt{3}}{16} L_{\rm in} (n+1)
 +\big( \frac{5}{3}+\frac{\pi\sqrt{3}}{36}\big) |(x_1,y_1,z_1)-(x_2,y_2,z_2)|
   \nonumber \\
&\leq  \big( \frac{\sqrt{3}}{48} +\frac{5}{3}
 +\frac{\pi\sqrt{3}}{36} \big) |(x_1,y_1,z_1)-(x_2,y_2,z_2)|. \nonumber 
\end{align}
Combining \eqref{eq:4.66} and \eqref{eq:4.67}, we have
\begin{equation}\begin{split}\label{eq:4.68}
&\operatorname{dist} (p,\partial \Omega_{\rm out} (n)\times \mathbb{R})\\
&\geq  \frac{1}{4} \Big( \frac{1}{4} +\frac{\pi}{3} \Big)^{-1}
\Big( \frac{\sqrt{3}}{48} +\frac{5}{3} +\frac{\pi \sqrt{3}}{36}
 \big)^{-1} |(x_1,y_1,z_1)-(x_2,y_2,z_2)|^{-1}\\
&\quad \times |p-(x_1,y_1,z_1)| |p-(x_2,y_2,z_2)|.
\end{split}\end{equation}
Now let $p\in \Gamma (x_2,y_2)\times \{ z_2\}$.
Let $k_1>0$ be the constant defined in \eqref{eq:4.21}.
Then calculations similar to those in \eqref{eq:4.22} give
\begin{equation}\label{eq:4.69}
\operatorname{dist} (p,\partial \Omega_{\rm out} (n)\times \mathbb{R})
\geq k_1 |p-(x_2,y_2,z_2)|.
\end{equation}
Also, by \eqref{eq:4.2},
\begin{equation}\begin{split}\label{eq:4.70}
|p-(x_1,y_1,z_1)|
&\leq  |p-(x_2,y_2,z_2)|+|(x_2,y_2,z_2)-(x_1,y_1,z_1)|\\
&\leq  \frac{\pi \sqrt{3}}{12} L_{\rm in} (n+1)+|(x_1,y_1,z_1)-(x_2,y_2,z_2)|\\
&\leq  \big(\frac{\pi\sqrt{3}}{36}+1\big)
|(x_1,y_1,z_1)-(x_2,y_2,z_2)|.
\end{split}\end{equation}
Combining \eqref{eq:4.69} and \eqref{eq:4.70} we obtain
\begin{equation}\begin{split}\label{eq:4.71}
\operatorname{dist} (p,\partial \Omega_{\rm out} (n)\times \mathbb{R})
&\geq  k_1 \Big( \frac{\pi\sqrt{3}}{36} +1\Big)^{-1}
|(x_1,y_1,z_1) -(x_2,y_2,z_2)|^{-1}\\
&\times |p-(x_1,y_1,z_1)| |p-(x_2,y_2,z_2)|.
\end{split}\end{equation}
Let $p\in \Gamma (x_1,y_1)\times \{ z_1\}$.
Then \eqref{eq:4.36} and \eqref{eq:4.37}, and their proofs, still hold.
 Thus we have
\begin{equation}\begin{split} \label{eq:4.72}
\operatorname{dist} (p,\partial \Omega_{\rm out} (n)\times \mathbb{R})
&\geq  \frac{3}{4} \min \{\cos \beta _1,k_2\} |(x_1,y_1,z_1)-(x_2,y_2,z_2)|^{-1}\\
&\quad \times |p-(x_1,y_1,z_1)||p-(x_2,y_2,z_2)|,
\end{split}\end{equation}
where $\beta_1$ and $k_2$ are constants described in Case~1(ii).

 Thus from \eqref{eq:4.5}, \eqref{eq:4.6}, \eqref{eq:4.57},
\eqref{eq:4.58}, \eqref{eq:4.59}, \eqref{eq:4.63}, \eqref{eq:4.64},
\eqref{eq:4.68}, \eqref{eq:4.71} and \eqref{eq:4.78},
 we see that if $(x_1, y_1, z_1)$ and $(x_2, y_2, z_2)$ satisfy the
assumptions of Case~1(iii) and if
\[
|(x_1,y_1,z_1)-(x_2,y_2,z_2)|\leq \hat{\delta }/3,
\]
then there exists a path
\begin{equation}\label{eq:4.73}
 \tilde{\Gamma} =(\Gamma (x_1,y_1)\times \{z_1\})+\Gamma
+(\Gamma (x_2,y_2)\times \{ z_2\})
\end{equation}
joining $(x_1,y_1,z_1)$ to $(x_2,y_2,z_2)$ satisfying
\begin{equation} \label{eq:4.74}
\operatorname{length}(\tilde{\Gamma})
\leq  \big[ \frac{1}{3} +\frac{\pi\sqrt{3}}{36} +\hat{\epsilon }^{-1}
\big( \frac{4}{3}+\frac{\pi\sqrt{3}}{36} \big) \big]
|(x_1,y_1,z_1) -(x_2,y_2,z_2)|
\end{equation}
and for all $p\in \tilde{\Gamma}$ we have
\begin{equation}\begin{split}\label{eq:4.75}
&\operatorname{dist} (p,\partial \Omega_{\rm out} (n)\times \mathbb{R})\\
&\geq  \epsilon_3 |(x_1,y_1,z_1)-(x_2,y_2,z_2)|^{-1}
|p-(x_1,y_1,z_1)| |p-(x_2,y_2,z_2)|
\end{split}\end{equation}
where
\begin{equation}\begin{split}\label{eq:4.76}
\epsilon_3
&= \min \Big\{ \hat{\epsilon}
 \Big( \frac{4}{3} +\frac{\pi\sqrt{3}}{36} \Big)^{-1}
 (1+4\sqrt{3})^{-1} \Big( 1+\frac{4\pi}{3}\Big)^{-1}, \\
&\quad \frac{1}{4\sqrt{3}} \Big( \frac{1}{4\sqrt{3}} +1\Big)^{-1}
\Big[ \big( \frac{1}{4\sqrt{3}} +1 \big) 3^{-1} +1\Big]^{-1},\\
&\quad \frac{1}{4} \Big( \frac{1}{4} +\frac{\pi}{3} \Big)^{-1}
\Big( \frac{\sqrt{3}}{48}+\frac{5}{3} +\frac{\pi\sqrt{3}}{36}\Big)^{-1},  k_1\left( \frac{\pi \sqrt{3}}{36} +1\right)^{-1},\\
&\quad \frac{3}{4} \cos \beta_1,  \frac{3}{4} k_2\Big\}.
\end{split}\end{equation}

\subsection*{Case 2(i)}
Here we assume that $(x_1,y_1)\in \Omega_{\rm out} (n)\backslash
\Omega_{\rm in} (n+1)$ and $(x_2,y_2)\in \Omega_{\rm in} (n+1)$, that
$(x_1,y_1)$ and $(x_2,y_2)$ are not both inside a region
$R\subseteq \Omega_{\rm out} (n)$ which is obtained from the polygon $S$
in Figure~\ref{fig1} by a finite sequence of dilations and
isometries and that some of the edges of $R$ are also edges
of $\Omega_{\rm out} (n)$, that $(x_1,y_1)$ is within a distance
of $\frac{1}{2}\cos (\pi/6) L_{\rm in} (n+1)$ from an acute vertex
$v_1$ of $\Omega_{\rm in} (n+1)$, and that \eqref{eq:4.4}
and \eqref{eq:4.5} hold.

 By Proposition~\ref{prop:4.2} there exists a path
$\Gamma \subseteq \Omega_{\rm in} (n+1)\times \mathbb{R}$
joining $(a(x_1,y_1),z_1)$ to $(x_2,y_2,z_2)$ satisfying
\begin{itemize}
\item[(C)] $\operatorname{length}(\Gamma )\leq \hat{\epsilon}^{-1}
|(a(x_1,y_1),z_1)-(x_2,y_2,z_2)|$,
\item[(D)] for all $p\in \Gamma$ we have
\begin{equation}\begin{split}\label{eq:4.77}
&\operatorname{dist} (p, \partial \Omega_{\rm in} (n+1) \times \mathbb{R})\\
&\geq  \hat{\epsilon} |(a(x_1,y_1),z_1)-(x_2,y_2,z_2)|^{-1}
 |p-(a(x_1,y_1),z_1)| |p-(x_2,y_2,z_2)|.
\end{split}\end{equation}
\end{itemize}
By \eqref{eq:4.2}, we have
\begin{equation}\begin{split}\label{eq:4.78}
&|(a(x_1,y_1),z_1)-(x_2,y_2,z_2)|\\
&\leq  |(a(x_1,y_1),z_1)-(x_1,y_1,z_1)|+|(x_1,y_1,z_1)-(x_2,y_2,z_2)|\\
&\leq  \frac{\pi\sqrt{3}}{12} L_{\rm in} (n+1)+|(x_1,y_1,z_1)-(x_2,y_2,z_2)|\\
&\leq  \big( \frac{\pi\sqrt{3}}{36} +1\big) |(x_1,y_1,z_1)-(x_2,y_2,z_2)|\end{split}\end{equation}
and
\begin{align*}
&|(x_1,y_1,z_1)-(x_2,y_2,z_2)|\\
&\leq  |(x_1,y_1,z_1)-(a(x_1,y_1),z_1)|+|(a (x_1,y_1),z_1) - (x_2,y_2,z_2)|\\
&\leq  \frac{\pi\sqrt{3}}{36} |(x_1,y_1,z_1) -(x_2,y_2 ,z_2)|
+ |(a(x_1,y_1),z_1)-(x_2,y_2,z_2)|
\end{align*}
and hence
\begin{equation}\label{eq:4.79}
|(x_1,y_1,z_1) - (x_2,y_2,z_2)|\leq
\Big( 1-\frac{\pi\sqrt{3}}{36} \Big)^{-1}
|(a(x_1,y_1),z_1)-(x_2,y_2,z_2)|.
\end{equation}
Thus
\begin{equation}\begin{split}\label{eq:4.80}
\operatorname{length}(\Gamma )
&\leq \hat{\epsilon}^{-1} |(a(x_1,y_1),z_1) -(x_2,y_2,z_2)|\\
&\leq \hat{\epsilon}^{-1} \big(\frac{\pi\sqrt{3}}{36} +1\big)
|(x_1,y_1,z_1)-(x_2,y_2,z_2)|
\end{split}\end{equation}
and
\begin{equation}\begin{split}\label{eq:4.81}
 \operatorname{length}(\Gamma (x_1,y_1)\times \{ z_1\})
&=\operatorname{length}(\Gamma (x_1,y_1))\\
&\leq \frac{\pi \sqrt{3}}{12} L_{\rm in} (n+1)\\
&\leq \frac{\pi \sqrt{3}}{36} |(x_1,y_1,z_1)-(x_2,y_2,z_2)|.
\end{split}\end{equation}
Let $p=(x,y,z_1) \in \Gamma (x_1,y_1)\times \{ z_1\}$.
Let $k_1>0$ be the constant defined by \eqref{eq:4.21}.
Then \eqref{eq:4.22} and \eqref{eq:4.23} still hold, and hence we
have
\begin{equation}\begin{split} \label{eq:4.82}
\operatorname{dist} (p,\partial \Omega_{\rm out} (n)\times \mathbb{R})
&\geq  k_1\Big( \frac{\pi\sqrt{3}}{36} +1\Big)^{-1} |(x_1,y_1,z_1)-(x_2,y_2,z_2)|^{-1}\\
&\times |p-(x_1,y_1,z_1)| |p-(x_2,y_2,z_2)|.
\end{split}\end{equation}
Let $p\in \Gamma$ and suppose that
\[
|p-(a(x_1,y_1),z_1)| \geq \frac{1}{2} \operatorname{dist} (a(x_1,y_1),
\partial \Omega _{\rm in} (n+1)).
\]
Then
\begin{align*}
|p-(a(x_1,y_1),z_1)|&\geq \frac{1}{2}\sin (\pi/6) |a(x_1,y_1)-v_1|\\
&=\frac{3}{4\pi} \left( \frac{\pi}{3} |a(x_1,y_1)-v_1|\right)\\
&\geq \frac{3}{4\pi} |(a(x_1,y_1),z_1)-(x_1,y_1,z_1)|,
\end{align*}
hence
\begin{equation}\begin{split}\label{eq:4.83}
 |p-(x_1,y_1,z_1) |&\leq |p-(a(x_1,y_1),z_1)|
+ |(a(x_1,y_1),z_1)-(x_1,y_1,z_1)|\\
&\leq \big( 1+\frac{4\pi}{3} \big) |p-(a(x_1,y_1),z_1)|.
\end{split}\end{equation}
Combining \eqref{eq:4.80} and \eqref{eq:4.83} we have
\begin{equation}\begin{split}\label{eq:4.84}
&\operatorname{dist} (p,\partial \Omega_{\rm out} (n)\times \mathbb{R})\\
&\geq  \operatorname{dist} (p,\partial \Omega_{\rm in} (n+1)\times \mathbb{R})\\
&\geq  \hat{\epsilon} |(a(x_1,y_1),z_1) -(x_2,y_2,z_2)|^{-1}
|p-(a(x_1,y_1),z_1)|  |p-(x_2,y_2,z_2)|\\
&\geq  \hat{\epsilon}\Big( \frac{\pi \sqrt{3}}{36} +1\Big)^{-1}
\Big( 1+\frac{4\pi}{3}\Big)^{-1} |(x_1,y_1,z_1)-(x_2,y_2,z_2)|^{-1}\\
&\times |p-(x_1,y_1,z_1)| |p-(x_2,y_2,z_2)|.
\end{split}\end{equation}
Next let $p\in \Gamma$ and suppose that
\[
|p-(a(x_1,y_1),z_1)|<\frac{1}{2} \operatorname{dist} (a(x_1,y_1),
\partial \Omega_{\rm in} (n+1)).\]
Then
\begin{equation}\begin{split} \label{eq:4.85}
|p-(x_1,y_1,z_1)|&\leq |p-(a(x_1,y_1),z_1) |+|(a(x_1,y_1),z_1 )
 -(x_1,y_1,z_1)|\\
&\leq \frac{1}{4} |a(x_1,y_1)-v_1|+\frac{\pi}{3} |a(x_1,y_1)-v_1|\\
&= \big( \frac{1}{4} +\frac{\pi}{3} \big) |a(x_1,y_1)-v_1|,
\end{split}\end{equation}
and so
\begin{equation}\begin{split}\label{eq:4.86}
\operatorname{dist} (p,\partial \Omega_{\rm out} (n)\times \mathbb{R})
&\geq  \operatorname{dist} (p,\partial \Omega_{\rm in} (n+1)\times \mathbb{R})\\
&\geq  \frac{1}{2} \operatorname{dist} (a(x_1,y_1),\partial \Omega_{\rm in} (n+1))\\
&=  \frac{1}{4} |a(x_1,y_1)-v_1|\\
&\geq  \frac{1}{4} \big( \frac{1}{4} +\frac{\pi}{3}\big)^{-1}
|p-(x_1,y_1,z_1)|.
\end{split}\end{equation}
Also we have, by \eqref{eq:4.80} and \eqref{eq:4.2},
\begin{equation}\begin{split}\label{eq:4.87}
&|p-(x_2,y_2,z_2)|\\
&\leq  |p-(a(x_1,y_1),z_1)| + |(a(x_1,y_1),z_1) -(x_2,y_2,z_2)|\\
&\leq  \frac{1}{4} |a(x_1,y_1)-v_1 |
 +\big( \frac{\pi\sqrt{3}}{36} +1\big) |(x_1,y_1,z_1)- (x_2,y_2,z_2)|\\
&\leq  \frac{\sqrt{3}}{16} L_{\rm in} (n+1)
 +\big( \frac{\pi\sqrt{3}}{36} +1\big) |(x_1,y_1,z_1)-(x_2,y_2,z_2)|\\
&\leq  \big( \frac{\sqrt{3}}{48} +\frac{\pi\sqrt{3}}{36} +1\big)
 |(x_1,y_1,z_1)-(x_2,y_2,z_2)|.
\end{split}\end{equation}
Combining \eqref{eq:4.86} and \eqref{eq:4.87} we obtain
\begin{equation}\begin{split}\label{eq:4.88}
&\operatorname{dist} (p,\partial \Omega_{\rm out} (n)\times \mathbb{R})\\
&\geq  \frac{1}{4} \Big( \frac{1}{4} +\frac{\pi}{3} \Big)^{-1}
 \Big( \frac{\sqrt{3}}{48} +\frac{\pi\sqrt{3}}{36} +1\Big)^{-1}
 |(x_1,y_1,z_1)-(x_2,y_2,z_2)|^{-1}\\
&\quad \times |p-(x_1,y_1,z_1)||p-(x_2,y_2,z_2)|.
\end{split}\end{equation}
Thus from \eqref{eq:4.5}, \eqref{eq:4.6}, \eqref{eq:4.80},
\eqref{eq:4.81}, \eqref{eq:4.82}, \eqref{eq:4.84}, and
\eqref{eq:4.88}, we see that if $(x_1,y_1,z_1)$ and
 $(x_2,y_2,z_2)$ satisfy the assumptions of Case~2(i) and if
\[
|(x_1,y_1,z_1)-(x_2,y_2,z_2)|\leq \hat{\delta}/3,
\]
then there exists a path
\begin{equation}\label{eq:4.89}
\tilde{\Gamma} =(\Gamma (x_1,y_1)\times \{z_1\} )+\Gamma
\end{equation}
joining $(x_1,y_1,z_1)$ to $(x_2,y_2,z_2)$ satisfying
\begin{equation}\label{eq:4.90}
\operatorname{length}(\tilde{\Gamma})
\leq \Big( \frac{\pi\sqrt{3}}{36} +\hat{\epsilon}^{-1}
\big( \frac{\pi\sqrt{3}}{36} +1\big)\Big)
 |(x_1,y_1,z_1)-(x_2,y_2,z_2)|
\end{equation}
and for all $p\in \tilde{\Gamma}$ we have
\begin{equation}\begin{split} \label{eq:4.91}
&\operatorname{dist} (p,\partial \Omega_{\rm out} (n)\times \mathbb{R})\\
&\geq   \epsilon_4 |(x_1,y_1,z_1)-(x_2,y_2,z_2)|^{-1}
|p-(x_1,y_1,z_1) ||p-(x_2,y_2,z_2)|
\end{split}\end{equation}
where
\begin{equation}\begin{split}
\epsilon_4 &= \min \Big\{ k_1 \Big( \frac{\pi \sqrt{3}}{36}+1\Big)^{-1},
 \hat{\epsilon} \Big( \frac{\pi \sqrt{3}}{36} +1\Big)^{-1}
\Big( 1+\frac{4\pi}{3} \Big)^{-1},\\
&\quad  \frac{1}{4} \Big( \frac{1}{4} +\frac{\pi}{3}\Big)^{-1}
\Big( \frac{\sqrt{3}}{48} +\frac{\pi \sqrt{3}}{36} +1\Big)^{-1}
 \Big\}.
\end{split}\end{equation}

\subsection*{Case 2(ii)}
Here we assume that $(x_1,y_1)\in \Omega_{\rm out}(n)\backslash
\Omega _{\rm in} (n+1)$ and $(x_2,y_2)\in \Omega_{\rm in} (n+1)$,
that $(x_1,y_1)$ and $(x_2,y_2)$ are not both inside a region
$R\subseteq \Omega_{\rm out} (n)$ which is obtained from the polygon
$S$ in Figure~\ref{fig1} by a finite sequence of dilations
and isometries and that some of the edges of $R$ are also edges
 of $\Omega_{\rm out} (n)$, that $(x_1,y_1)$ is not within a distance
of $\frac{1}{2}\cos (\pi/6)L_{\rm in} (n+1)$ from any acute vertex
of $\Omega_{\rm in} (n+1)$, and that \eqref{eq:4.4} and
\eqref{eq:4.5} holds.

 Referring to Figure~\ref{fig5}, we see that in this case
\eqref{eq:4.31}-\eqref{eq:4.38} and \eqref{eq:4.40} still hold,
and so, for all $p\in \Gamma (x_1,y_1)\times \{ z_1\}$, we have
\begin{equation}\begin{split}\label{eq:4.93}
\operatorname{dist} (p,\partial \Omega_{\rm out} (n)\times \mathbb{R})
&\geq  \frac{3}{4} \min\{\cos \beta_1 ,k_2\} |(x_1,y_1,z_1) - (x_2,y_2,z_2)|^{-1}\\
&\quad \times |p-(x_1,y_1,z_1)| |p-(x_2,y_2,z_2)|,
\end{split}\end{equation}
and
\begin{equation}\label{eq:4.94}
 \operatorname{length}(\Gamma (x_1,y_1)\times \{z_1\} )
\leq \frac{1}{3} |(x_1,y_1,z_1)-(x_2,y_2,z_2)|.\end{equation}
Hence
\begin{equation}\begin{split}\label{eq:4.95}
&\operatorname{length}(\Gamma)\\
&\leq  \hat{\epsilon}^{-1} |(a(x_1,y_1),z_1)-(x_2,y_2,z_2)|\\
&\leq  \hat{\epsilon}^{-1} \{ |(a(x_1,y_1),z_1)-(x_1,y_1,z_1)| +|(x_1,y_1,z_1)- (x_2,y_2,z_2)|\}\\
&\leq  \frac{4}{3} \hat{\epsilon}^{-1} |(x_1,y_1,z_1) -(x_2,y_2,z_2)|.
\end{split}\end{equation}
Let $p\in \Gamma$ and suppose that
\[
|p-(a(x_1,y_1),z_1)|\geq \frac{1}{2} \operatorname{dist} (a(x_1,y_1),
\partial \Omega_{\rm in} (n+1)).
\]
Then
\begin{equation} \label{eq:4.96}
|p-(a(x_1,y_1),z_1)|\geq  \frac{1}{4\sqrt{3}} L_{\rm in} (n+1)
\geq  \frac{1}{4\sqrt{3}} |(a(x_1,y_1),z_1) -(x_1,y_1,z_1)|.
\end{equation}
Thus
\begin{equation}\begin{split}\label{eq:4.97}
|p-(x_1,y_1,z_1)|&\leq |p-(a(x_1,y_1),z_1)|
 +|(a(x_1,y_1),z_1)-(x_1,y_1,z_1)|\\
&\leq (1+4\sqrt{3})|p-(a(x_1,y_1),z_1)|.
\end{split}\end{equation}
Also, from \eqref{eq:4.2} and Figure~\ref{fig5},
\begin{equation}\begin{split}\label{eq:4.98}
&|(a(x_1,y_1),z_1) -(x_2,y_2,z_2)|\\
&\leq  |(a(x_1,y_1),z_1)-(x_1,y_1,z_1)| + |(x_1, y_1, z_1) - (x_2, y_2, z_2)|\\
&\leq  L_{\rm in} (n+1) +|(x_1,y_1,z_1)-(x_2,y_2,z_2)|\\
&\leq  \frac{4}{3} |(x_1,y_1,z_1) -(x_2,y_2,z_2)|.
\end{split}\end{equation}
Hence we have, from \eqref{eq:4.97} and \eqref{eq:4.98},
\begin{equation}\begin{split}\label{eq:4.99}
\operatorname{dist} (p,\partial \Omega_{\rm out} (n)\times \mathbb{R})
 &\geq  \operatorname{dist} (p,\partial \Omega_{\rm in} (n+1)\times \mathbb{R})\\
 &\geq  \hat{\epsilon} |(a(x_1,y_1),z_1)-(x_2,y_2,z_2)|^{-1} |p-(a(x_1,y_1),z_1)|\\
&\times |p-(x_2,y_2,z_2)|\\
&\geq  \hat{\epsilon} \frac{3}{4} (1+4\sqrt{3} )^{-1} |(x_1,y_1,z_1)-(x_2,y_2,z_2)|^{-1}\\
&\times |p-(x_1,y_1,z_1)| |p-(x_2,y_2,z_2)|.
\end{split}\end{equation}
Now let $p\in \Gamma$ and suppose that
\[
|p-(a(x_1,y_1) ,z_1)|<\frac{1}{2} \operatorname{dist} (a(x_1,y_1),
\partial \Omega_{\rm in} (n+1)).
\]
Then
\begin{equation}\begin{split}\label{eq:4.100}
 \operatorname{dist} (p,\partial \Omega_{\rm out} (n)\times \mathbb{R})
&\geq  \operatorname{dist} (p,\partial \Omega_{\rm in} (n+1)\times \mathbb{R})\\
&\geq  \frac{1}{2} \operatorname{dist} ((a(x_1,y_1),z_1),\partial \Omega_{\rm in} (n+1)\times \mathbb{R})\\
&=  \frac{1}{4\sqrt{3}} L_{\rm in} (n+1)
\end{split}\end{equation}
and, referring to Figure~\ref{fig5},
\begin{equation}\begin{split}\label{eq:4.101}
|p-(x_1,y_1,z_1)|&\leq |p-(a(x_1,y_1),z_1)|
+ |(a(x_1,y_1),z_1) -(x_1,y_1,z_1)|\\
&\leq \big( \frac{1}{4\sqrt{3}} +1\big) L_{\rm in} (n+1).
\end{split}\end{equation}
Hence, combining \eqref{eq:4.100} and \eqref{eq:4.101}, we get
\begin{equation}\label{eq:4.102}
\operatorname{dist} (p,\partial \Omega_{\rm out} (n)\times \mathbb{R})
\geq \frac{1}{4\sqrt{3}} \Big(\frac{1}{4\sqrt{3}} +1\Big)^{-1}
|p-(x_1,y_1,z_1)|.
\end{equation}
Also, by \eqref{eq:4.2} and \eqref{eq:4.101},
\begin{equation}\begin{split}\label{eq:4.103} |p-(x_2,y_2,z_2)|
&\leq |p-(x_1,y_1,z_1)|+|(x_1,y_1,z_1)-(x_2,y_2,z_2)|\\
&\leq \big( \frac{1}{4\sqrt{3}}+1\big) L_{\rm in} (n+1)+|(x_1,y_1,z_1)-(x_2,y_2,z_2)|\\
&\leq \big( \frac{1}{12\sqrt{3}}+\frac{4}{3}\big)
|(x_1,y_1,z_1)-(x_2,y_2,z_2)|.
\end{split}\end{equation}
Combining \eqref{eq:4.102} and \eqref{eq:4.103} we obtain
\begin{equation}\begin{split}\label{eq:4.104}
&\operatorname{dist} (p,\partial \Omega_{\rm out} (n)\times \mathbb{R})\\
&\geq  \frac{1}{4\sqrt{3}} \Big( \frac{1}{4\sqrt{3}}+1\big)^{-1}
 \Big( \frac{1}{12\sqrt{3}} +\frac{4}{3}\Big)^{-1} |(x_1,y_1,z_1)-(x_2,y_2,z_2)|^{-1}\\
&\quad \times |p-(x_1,y_1,z_1)| |p-(x_2,y_2,z_2)|.
\end{split}\end{equation}
Thus from \eqref{eq:4.5}, \eqref{eq:4.6}, \eqref{eq:4.93},
\eqref{eq:4.94}, \eqref{eq:4.95}, \eqref{eq:4.99}, and
\eqref{eq:4.104}, we see that if $(x_1,y_1,z_1)$ and $(x_2,y_2,z_2)$
 satisfy the assumptions of Case~2(ii) and if
\[
|(x_1,y_1,z_1)-(x_2,y_2,z_2)|\leq \hat{\delta}/3,
\]
then there exists a path
\begin{equation}\label{eq:4.105}
\tilde{\Gamma} =(\Gamma (x_1,y_1)\times \{ z_1\})+\Gamma
\end{equation}
joining $(x_1,y_1,z_1)$ to $(x_2,y_2,z_2)$ satisfying
\begin{equation}\label{eq:4.106}
\operatorname{length}(\tilde{\Gamma}) \leq
\big( \frac{1}{3} +\frac{4}{3} \hat{\epsilon}^{-1}\big)
|(x_1,y_1,z_1)-(x_2,y_2,z_2)|
\end{equation}
and for all $p\in \tilde{\Gamma}$ we have
\begin{equation}\begin{split}\label{eq:4.107}
&\operatorname{dist} (p,\partial \Omega_{\rm out} (n)\times \mathbb{R})\\
&\geq  \epsilon_5 |(x_1,y_1,z_1)-(x_2,y_2,z_2)|^{-1}
|p-(x_1,y_1,z_1)| |p-(x_2,y_2,z_2)|
\end{split}\end{equation}
where
\begin{equation}\begin{split}\label{eq:4.108}
 \epsilon_5&= \min\Big\{ \frac{3}{4}\cos \beta_1,
 \frac{3}{4} k_2,  \frac{3}{4} \big(1 +4\sqrt{3}\big)^{-1}
\hat{\epsilon},\\
&\quad  \frac{1}{4\sqrt{3}} \Big( \frac{1}{4\sqrt{3}} +1\Big)^{-1}
 \Big( \frac{1}{12\sqrt{3}} +\frac{4}{3}\Big)^{-1} \Big\}.
\end{split}\end{equation}

 To summarize: Cases~1(i),(ii),(iii), 2(i),(ii), exhaust all
possibilities of at least one of $(x_1,y_1,z_1)$ or
$(x_2,y_x,z_2)$ is in $(\Omega_{\rm out} (n)\times
\mathbb{R})\backslash (\Omega_{\rm in} (n+1)\times \mathbb{R})$
with $(x_1,y_1)$ and $(x_2,y_2)$ not both contained in a region
$R\subseteq \Omega _{\rm out} (n)$ which is obtained from the polygon
$S$ in Figure~\ref{fig1}  by a finite sequence of dilations and
isometries and that at least one of the edges of $R$ is also an
edge of $\Omega_{\rm out} (n)$. Let
\begin{equation}\label{eq:4.109}
\delta_6 =\hat{\delta} /3
\end{equation}
and
\begin{equation}\begin{split}\label{eq:4.110}
\epsilon_6 &= \min \Big\{ \Big[ \frac{\sqrt{3}\pi}{18}
+\hat{\epsilon} \big( \frac{\sqrt{3}\pi}{18} +1\big)\Big]^{-1},
 \Big( \frac{2}{3} +\frac{5}{3}\hat{\epsilon}^{-1} \Big)^{-1}, \\
&\quad \Big[\frac{1}{3} +\frac{\pi\sqrt{3}}{36}
 +\hat{\epsilon}^{-1} \big( \frac{4}{3} +\frac{\pi\sqrt{3}}{36} \big)
 \Big]^{-1} ,\Big[ \frac{\pi\sqrt{3}}{36} +\hat{\epsilon}^{-1}
 \Big(\frac{\pi\sqrt{3}}{36} +1\Big)\Big]^{-1},\\
&\quad  \Big( \frac{1}{3} +\frac{4}{3}
\hat{\epsilon}^{-1}\Big)^{-1}, \epsilon_1, \epsilon_2, \,
\epsilon_3,  \epsilon_4, \epsilon_5\Big\}.
\end{split}\end{equation}
Then we have proved that in each of these cases, if
\begin{equation}\label{eq:4.111}
|(x_1,y_1,z_1)-(x_2,y_2,z_2)|\leq \delta _6,
\end{equation}
then there exists a path $\tilde{\Gamma} \subseteq \Omega_{\rm out}
(n)\times \mathbb{R}$ joining $(x_1,y_1,z_1)$ to $(x_2,y_2,z_2)$
satisfying
\begin{equation}\label{eq:4.112}
\operatorname{length}(\tilde{\Gamma})
\leq \epsilon_6^{-1} |(x_1,y_1,z_1) -(x_2,y_2,z_2)|
\end{equation}
and for all $p\in \tilde{\Gamma}$ we have
\begin{equation}\begin{split}\label{eq:4.113}
&\operatorname{dist} (p,\partial \Omega_{\rm out} (n)\times \mathbb{R})\\
&\geq  \epsilon_6 |(x_1,y_1,z_1)-(x_2,y_2,z_2)|^{-1}
|p-(x_1,y_1,z_1)| |p-(x_2,y_2,z_2)|.
\end{split}\end{equation}
This together with Proposition~\ref{prop:4.2} and the fact
$S\times \mathbb{R}$ is a Lipschitz domain, and thus an
$(\epsilon_7,\delta_7)$-domain in $\mathbb{R}^3$ for some
$\epsilon_7,\delta_7>0$, complete the proof of Theorem~\ref{thm:4.3}.
\end{proof}

 We finish this section by giving the proof of Theorem~\ref{thm:1.3}.
We shall need the following results:

\begin{proposition}[{see \cite[Theorem 1]{J}}]\label{prop:4.4}
 Let $D\in \mathbb{R}^d$ be an $(\epsilon,\delta)$-domain.
Suppose $k\in \{1,2,3,\dots \}$ and $1\leq p\leq \infty$.
Then there exists a bounded extension operator
$\Lambda_{k,p}:W^{k,p} (D)\to W^{k,p} (\mathbb{R}^d)$ such that
\[
(\Lambda_{k,p} f)|_D \,=f\quad (f\in W^{k,p}(D)).
\]
Moreover, the norm $\| \Lambda_{k,p}\|$ depends only on
$\epsilon $, $\delta$, $k$, $p$ and the dimension $d$.
\end{proposition}

\begin{proposition}[{see \cite[p.47]{D2}}] \label{prop:4.5}
Suppose $D\subseteq \mathbb{R}^d$ is a domain such that for some
$p\in [1,d)$ there exists a bounded extension operator
$\Lambda_{1,p}:W^{1,p} (D)\to W^{1,p} (\mathbb{R}^d)$ satisfying
\[
(\Lambda_{1,p} f)|_D\,=f\quad (f\in W^{1,p}(D)).
\]
Let $q$ be defined by $\frac{1}{q}=\frac{1}{p}-\frac{1}{d}$. Then
there exists $c=c(d)\geq 1$ such that
\[
\| f\|_q\leq c\|\Lambda_{1,p} \| \{ \| \nabla f\|^p_p
+\| f\|^p_p\} ^{\frac{1}{p}}\quad (f\in W^{1,p}(D)).
\]
\end{proposition}

\begin{proposition}
[{see \cite[Theorem 2.4.2, Corollaries 2.4.3,and 2.2.8]{D2}}]
\label{prop:4.6}
Let $D\subseteq \mathbb{R}^d$, $d\geq 3$, be a domain. Suppose
there exists $c_1\geq 1$ such that
\[
 \| f\|_{\frac{2d}{d-2}} \leq c_1 \{ \|\nabla f\|^2_2
+\| f\|^2_2\} ^{1/2} \quad (f\in W^{1,2} (D)).
\]
Then there exists $c_2\geq 1$, depending only on $c_1$ and $d$, such
that
\[
P^D(t,x,y)\leq c_2t^{-d/2}\quad (0<t\leq 1, x,y\in D),
\]
where $P^D(t,x,y)$ denotes the heat kernel associated to the
semigroup generated by the Neumann Laplacian on $D$.
\end{proposition}

\begin{proof}[Proof of Theorem~\ref{thm:1.3}]
We follow the arguments in \cite{P2}. We also remark that
the constants $K_i$, $i=1,2,3$, in the argument below will
depend only on the values of $\check{\epsilon}$ and
$\check{\delta}$ in Theorem~\ref{thm:4.3}, but not on $n$.

 By Theorem~\ref{thm:4.3} and Proposition~\ref{prop:4.4}
(with $D=\Omega_{\rm out} (n)\times \mathbb{R}$, $k=1$ and $p=2$
in Proposition~\ref{prop:4.4}), there exists a bounded
linear extension operator
$\Lambda_{1,2}: W^{1,2} (\Omega_{\rm out} (n)\times
\mathbb{R} )\to W^{1,2} (\mathbb{R}^3)$ such that
\[
(\Lambda_{1,2} f)\mid_{\Omega_{\rm out}(n)\times \mathbb{R}} =f\quad
(f\in W^{1,2}(\Omega_{\rm out} (n)\times \mathbb{R})),
\]
where the norm $\| \Lambda_{1,2}\|$ depends only on
$\check{\epsilon}$ and $\check{\delta}$.
So by Proposition~\ref{prop:4.5}
(with $D=\Omega_{\rm out} (n)\times \mathbb{R}$, $d=3$, $p=2$
and $q=6$), we have
\[
\| f\|_6 \leq K_1 \{ \| \nabla f\|^2_2 +\| f\|^2_2\}^{1/2}
\quad (f\in W^{1,2}(\Omega_{\rm out} (n)\times \mathbb{R}))
\]
where $K_1\geq 1$ depends only on $\check{\epsilon}$ and
$\check{\delta}$. Hence, by Proposition~\ref{prop:4.6}, we have
\begin{equation}\label{eq:4.114}
P^{\Omega_{\rm out} (n)\times \mathbb{R}} (t,(x_1,y_1,z_1) ,
(x_2,y_2,z_2))\leq K_2t^{-3/2}
\end{equation}
for all $0<t\leq 1$ and all $(x_1,y_1,z_1)$,
$(x_2,y_2,z_2)\in \Omega_{\rm out} (n)\times \mathbb{R}$,
where $K_2\geq 1$ depends only on $\check{\epsilon}$ and
$\check{\delta}$. Since
\begin{equation}\begin{split}\label{eq:4.115}
&P^{\Omega_{\rm out} (n)\times \mathbb{R}}
(t,(x_1,y_1,z), (x_2,y_2,z))\\
&=  P^{\Omega_{\rm out} (n)} (t,(x_1,y_1),(x_2,y_2))
P^{\mathbb{R}} (t,z,z)\\
&=  (4\pi t)^{-1/2} P^{\Omega_{\rm out} (n)}
(t,(x_1,y_1),(x_2,y_2))
\end{split}\end{equation}
for all $0<t\leq 1, (x_1,y_1), (x_2,y_2)\in \Omega_{\rm out} (n)$
and $z\in \mathbb{R}$, we have, from \eqref{eq:4.114} and
\eqref{eq:4.115},
\begin{equation}\label{eq:4.116}
P^{\Omega_{\rm out}(n)} (t,(x_1,y_1),(x_2,y_2))
\leq K_3t^{-1}
\end{equation}
for all $0<t\leq 1$ and $(x_1,y_1),(x_2,y_2)\in \Omega_{\rm out} (n)$,
where $K_3\geq 1$ depends only on $\check{\epsilon}$ and
$\check{\delta}$. The proof of Theorem~\ref{thm:1.3}
is complete by combining \eqref{eq:4.116} and \cite[Theorem~1.3]{P2}.
\end{proof}



\section*{Acknowledgement}
We thank the Summer Research Fellowship of the University of
Missouri for support during this project.


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\end{document}
