\documentclass[reqno]{amsart}
\usepackage{hyperref}
\usepackage{cite}

\AtBeginDocument{{\noindent\small
\emph{Electronic Journal of Differential Equations},
Vol. 2015 (2015), No. 76, pp. 1--28.\newline
ISSN: 1072-6691. URL: http://ejde.math.txstate.edu or http://ejde.math.unt.edu
\newline ftp ejde.math.txstate.edu}
\thanks{\copyright 2015 Texas State University - San Marcos.}
\vspace{9mm}}

\begin{document}
\title[\hfilneg EJDE-2015/76\hfil 
 Mixed interior and boundary peak solutions]
{Mixed interior and boundary peak solutions of the Neumann problem 
for the H\'enon equation \\ in $\mathbb{R}^2$}

\author[Y. Zhang, H. Yang \hfil EJDE-2015/76\hfilneg]
{Yibin Zhang, Haitao Yang}

\address{Yibin Zhang \newline
College of Sciences, Nanjing Agricultural University,
Nanjing 210095, China}
\email{yibin10201029@njau.edu.cn}

\address{Haitao Yang \newline
Department of Mathematics, Zhejiang University, 
Hangzhou 310027, China}
\email{htyang@css.zju.edu.cn}

\thanks{Submitted October 14, 2014. Published March 26, 2015.}
\subjclass[2000]{35J25, 35J20, 58K05}
\keywords{Mixed interior and boundary peak solutions;
H\'enon-type weight; \hfill\break\indent large exponent;
Lyapunov-Schmidt reduction process}

\begin{abstract}
 Let $\Omega$ be a bounded domain in $\mathbb{R}^2$ with smooth
 boundary and $0\in\overline{\Omega}$, we study the Neumann problem
 for the H\'enon equation
 \begin{gather*}
 -\Delta u+u=|x|^{2\alpha}u^p,\quad
 u>0 \quad \text{in } \Omega,\\
 \frac{\partial u}{\partial\nu}=0\quad \text{on } \partial\Omega,
 \end{gather*}
 where $\nu$ denotes the outer unit normal vector to $\partial\Omega$,
 $-1<\alpha\not\in\mathbb{N}\cup\{0\}$ and $p$ is a large exponent.
 In a constructive way,  we show that,  as $p$ approaches $+\infty$,
 such a problem has a family of positive solutions  with arbitrarily
 many interior and boundary spikes involving  the origin.
 The same techniques lead also to a more general result on
 H\'enon-type weights.
\end{abstract}

\maketitle
\numberwithin{equation}{section}
\newtheorem{theorem}{Theorem}[section]
\newtheorem{lemma}[theorem]{Lemma}
\newtheorem{proposition}[theorem]{Proposition}
\newtheorem{remark}[theorem]{Remark}
\allowdisplaybreaks


\section{Introduction}

In this article, we consider the Neumann  problem
\begin{equation}\label{a1}
\begin{gathered}
-\Delta u+u=S(x)u^p\quad \text{in } \Omega,\\
 u>0 \quad\text{in }\Omega,\\
 \frac{\partial u}{\partial\nu}=0\quad \text{on }\partial\Omega,
\end{gathered}
\end{equation}
where  $\Omega$ is a smooth  bounded   domain in $\mathbb{R}^2$,
$S$ is a nonnegative function on $\overline{\Omega}$,
$p$ is a large exponent and $\nu$ denotes the outer unit  normal
vector to  $\partial\Omega$.

It is well known that problem \eqref{a1} with $S\equiv1$ has a strong biological
meaning because it appears in the study of the   stationary  Keller-Segel
system with the logarithmic  sensitivity function from chemotaxis
(see \cite{KS,N1}):
\begin{equation}\label{a3}
\begin{gathered}
D_1\Delta v-\chi\nabla\cdot(v\nabla \log \omega)=0\quad\text{in }\Omega,\\
D_2\Delta \omega-a\omega+bv=0\quad\text{in } \Omega,\\
\frac{\partial \omega}{\partial \nu}
=\frac{\partial v}{\partial \nu}=0\quad \text{on } \partial\Omega,\\
\frac1{|\Omega|}\int_{\Omega}v(x)dx=\bar{v}>0\quad\text{(prescribed),}
\end{gathered}
\end{equation}
where $\Omega$ is a smooth  bounded domain in $\mathbb{R}^N(N\geq2)$
and the constants $D_1$, $D_2$, $a$, $b$ and $\chi$ are positive.
Indeed, it is easy to check that solutions of \eqref{a3} satisfy the relation
$$
\int_{\Omega}v|\nabla(\log v-p\log\omega)|^2=0\quad\text{where }p=\chi/D_1,
$$
so that $v=\lambda\omega^p$ for some positive constant $\lambda$. Thus, setting
$\varepsilon^2=D_2/a$, $\gamma=(b\lambda/a)^{\frac1{p-1}}$ and $u=\gamma\omega$,
we see that $u$ satisfies the singularly perturbed elliptic problem
\begin{equation}\label{a4}
\begin{gathered}
-\varepsilon^2\Delta u+u=u^p\quad \text{in }\Omega,\\
 u>0\quad \text{in } \Omega,\\
\frac{\partial u}{\partial\nu}=0\quad \text{on }\partial\Omega.
\end{gathered}
\end{equation}


In the pioneering papers \cite{LNT,NT1,NT2}, Lin, Ni and Takagi  proved
that for $\varepsilon>0$ sufficiently small and for $p>1$ subcritical
(more precisely, $1<p<(N+2)/(N-2)$ if $N\geq3$, and $1<p<+\infty$ if $N=2$),
problem \eqref{a4} has a least energy solution
 which develops a spike layer at the {\it most curved} part of the boundary,
i.e., the region where the mean curvature  attains  its maximum.
 Since then, there have
been many works looking for higher energy solutions of \eqref{a4} with multiple
boundary peaks as well as multiple interior peaks (see \cite{DFW,GW,GW1,GWW,L}
and references therein).
In particular, it was established  by  Gui and Wei in \cite{GW1}  that for any two
nonnegative integers
$m$, $\tilde{m}\geq0$, $m+\tilde{m}\geq1$, problem \eqref{a4} has a solution
with exactly $m$ interior spikes and $\tilde{m}$ boundary spikes provided that
$\varepsilon$ is small and $p$ is subcritical. In another direction, when
$N=2$ and $\varepsilon$ is finite (without loss of generality,
set  $\varepsilon=1$),  Musso and  Wei in \cite{MW1} considered another limit
 $p\to+\infty$ and  showed that for any two nonnegative integers
$m$, $\tilde{m}\geq0$, $m+\tilde{m}\geq1$, problem \eqref{a1} with $S\equiv1$
has also a solution with $m$ interior spikes and $\tilde{m}$ boundary spikes
provided that the exponent $p$ is large.

We are still looking for solutions of problem \eqref{a1} with multiple spikes
 both on the boundary and in the interior as the exponent  $p$ tends to $+\infty$.
A characteristic  feature of this paper is the presence of
the  function $S(x)$ in terms of the  weight
$|x|^{2\alpha}$ with $-1<\alpha\not\in\mathbb{N}\cup\{0\}$, originally
introduced by H\'enon in \cite{H} to study the rotating stellar structures.
 More precisely, we consider the Neumann problem for  the H\'enon equation
\begin{equation}\label{*}
\begin{gathered}
-\Delta u+u=|x|^{2\alpha}u^p\quad \text{in }\Omega,\\
u>0\quad \text{in } \Omega,\\
\frac{\partial u}{\partial\nu}=0\quad \text{on }\partial\Omega,
\end{gathered}
\end{equation}
where $\Omega$ is a smooth  bounded   domain in $\mathbb{R}^2$,
$0\in\overline{\Omega}$,  $-1<\alpha\not\in\mathbb{N}\cup\{0\}$,
$p$ is a large exponent and $\nu$ denotes the outer unit  normal
vector to  $\partial\Omega$.
Indeed,  the presence of the H\'enon-type weight
can produce significant influence on
the existence of a solution as well as its asymptotic behavior.
For this purpose, this paper is devoted to constructing solutions to
problem \eqref{*} with spike-layer profiles  at points inside
$\Omega$ and on the boundary of $\Omega$ involving the origin
when  $0\in\overline{\Omega}$ and $p$ tends to $+\infty$. In particular, we
recover the result in \cite{MW1} when $S\equiv1$.

For \eqref{*} we obtain the following result.

\begin{theorem} \label{thm1.1}
 Assume that $\Omega$ is a smooth
bounded domain in $\mathbb{R}^2$ and $0\in\overline{\Omega}$. Then for any
 $m,\tilde{m}\in\mathbb{N}\cup\{0\}$ and
for $p$ sufficiently large problem  \eqref{*}   has a positive solution
$u_p$  which concentrates at $m+\tilde{m}+1$ different  points
of $\overline{\Omega}$; i.e., as $p\to +\infty$,
$$
p|x|^{2\alpha}u^{p+1}_p\rightharpoonup
d_1e\delta_{0}+
8\pi e\sum_{i=2}^{m+1}\delta_{\tilde{q}_i}+
4\pi e\sum_{i=m+2}^{m+\tilde{m}+1}\delta_{\tilde{q}_i}
$$
weakly in the sense of measure in $\overline{\Omega}$,
for some points $\tilde{q}_{2},\ldots,\tilde{q}_{m+1}\in\Omega$
and  some points $\tilde{q}_{m+2},\ldots,\tilde{q}_{m+\tilde{m}+1}
\in\partial\Omega$,
where
$d_1=8\pi$ for $0\in\Omega$, and $d_1=4\pi$ for $0\in\partial\Omega$.
Furthermore, for  any $\delta>0$ sufficiently small,
\begin{gather*}
u_p\to0\quad \text{uniformly in } \overline{\Omega}\setminus
\cup_{i=2}^{m+\tilde{m}+1}B_{\delta}(\tilde{q}_i)\cup B_{\delta}(0),\\
\sup_{x\in\overline{\Omega}\cap B_{\delta}(0)}u_p(x)\to\sqrt{e},\quad
\sup_{x\in\overline{\Omega}\cap B_{\delta}(\tilde{q}_i)}u_p(x)\to\sqrt{e},
\end{gather*}
as $p\to+\infty$.
\end{theorem}

The above theorem is proved in a constructive way which also
works for the more general case
involving  the H\'enon-type weight with mixed interior and boundary
source points as follows:
\begin{equation}\label{a2}
S(x)=c(x)\prod_{i=1}^{n+\tilde{n}}|x-q_i|^{2\alpha_i},
\end{equation}
where $n+\tilde{n}\geq1$,
$q_1,\ldots,q_n\in\Omega$,
$q_{n+1},\ldots,q_{n+\tilde{n}}\in\partial\Omega$,
$-1<\alpha_1,\ldots,\alpha_{n+\tilde{n}}
\not\in\mathbb{N}\cup\{0\}$
and $c: \overline{\Omega}\to
\mathbb{R}$ is a continuous function satisfying
 $\inf_{\overline{\Omega}}c>0$, so that problem \eqref{a1} becomes
\begin{equation}\label{a}
\begin{gathered}
-\Delta u+u=c(x)\prod_{i=1}^{n+\tilde{n}}|x-q_i|^{2\alpha_i}u^p\quad \text{in } \Omega,\\
u>0\quad \text{in }\Omega,\\
\frac{\partial u}{\partial\nu}=0 \quad \text{on }\partial\Omega.
\end{gathered}
\end{equation}

Let us  first define the corresponding
Green's function for the Neumann problem
\begin{equation}\label{f}
\begin{gathered}
-\Delta_x G(x,y)+G(x,y)=\delta_y(x)\quad \text{in }\Omega,\\
 \frac{\partial G(x,y)}{\partial \nu_x}=0\quad\text{on }\partial\Omega.
\end{gathered}
\end{equation}
The regular part of $G(x,y)$ is defined depending on whether $y$ lies in
the domain or on its boundary as
\begin{equation}\label{f1}
H(x,y)=\begin{cases}
G(x,y)+\frac1{2\pi}\log|x-y|&\text{for}  y\in\Omega,\\
G(x,y)+\frac1{\pi}\log|x-y|&\text{for } y\in\partial\Omega.
\end{cases}
\end{equation}
In this way, $H(\cdot,y)$ is of class $C^{1,\beta}$ in $\overline{\Omega}$.


Next, for any nonnegative integers $m$ and $\tilde{m}$, we introduce
\begin{gather*}
J_1=\{1,\ldots,n\},\quad
J_2=\{n+1,\ldots,n+\tilde{n}\},\\
J_3=\{n+\tilde{n}+1,\ldots,n+\tilde{n}+m\},\quad
J_4=\{n+\tilde{n}+m+1,\dots,n+\tilde{n}+m+\tilde{m}\}.
\end{gather*}
Furthermore, we set
\begin{gather*}
\alpha_i=0\quad \text{for }i\in J_3\cup J_4,\\
c_i(x)=\frac{S(x)}{|x-q_i|^{2\alpha_i}}\quad \text{for }i\in\cup_{l=1}^4J_l,\\
d_i=\begin{cases}
8\pi(1+\alpha_i)&\text{for } i\in J_1\cup J_3,\\
4\pi(1+\alpha_i)&\text{for } i\in J_2\cup J_4.
\end{cases}
\end{gather*}
Also we define
\begin{gather*}
\Gamma_1=\{q_1,\ldots,q_n\},\quad
\Gamma_2=\{q_{n+1},\ldots,q_{n+\tilde{n}}\}, \\
\Lambda_{m}^{\tilde{m}}=(\Omega\setminus\Gamma_1)^m\times
(\partial\Omega\setminus\Gamma_2)^{\tilde{m}}\setminus\triangle_{m}^{\tilde{m}},
\end{gather*}
where $\triangle_{m}^{\tilde{m}}$ denotes the diagonal set.

Now, we  fix $n+\tilde{n}$
different source points $q_i$, $i\in J_1\cup J_2$.
For $\delta>0$ sufficiently small but fixed
 we define a configuration space
\begin{align*}
\Lambda_{m}^{\tilde{m}}(\delta)
=\big\{&(q_{n+\tilde{n}+1},\ldots,q_{n+\tilde{n}+m+\tilde{m}})\in
\Lambda_{m}^{\tilde{m}}: \operatorname{dist}(q_i,\partial\Omega)
\geq 2 \delta\; \forall i\in J_3;\\
&\operatorname{dist}(q_i,q_j)\geq2\delta\; forall i,j\in\cup_{l=1}^4J_l,\;i\neq j
\big\}.
\end{align*}
As a consequence,  for points
$q=(q_{n+\tilde{n}+1},\ldots,q_{n+\tilde{n}+m+\tilde{m}})
\in\Lambda_{m}^{\tilde{m}}(\delta)$,
if we set
\begin{equation}\label{b}
\begin{aligned}
\varphi_{m}^{\tilde{m}}(q)
&= \sum_{i\in J_3\cup J_4}d_i\Big\{2\log c_i(q_i)+d_iH(q_i,q_i)+
\sum_{j\in J_1\cup J_2}2d_jG(q_i,q_j)\\
&\quad + \sum_{j\in J_3\cup J_4,\,\,j\neq i}d_jG(q_i,q_j)
\Big\},
\end{aligned}
\end{equation}
we have the following theorem for \eqref{a}, which is the main
result of this article.

\begin{theorem} \label{thm1.2}
 Assume that $\Omega$ is a smooth
bounded domain in $\mathbb{R}^2$, $n+\tilde{n}\geq1$
 and $\inf_{\overline{\Omega}}c>0$. Then for any
 $m,\tilde{m}\in\mathbb{N}\cup\{0\}$ and
for $p$ sufficiently large
there exist different points
$q^p_l\in\Omega\setminus\Gamma_1$, $l\in J_3$,  and
$q^p_l\in\partial\Omega\setminus\Gamma_2$, $l\in J_4$,
 so that \eqref{a}  has a positive solution
$u_p$  which possesses  exactly $n+\tilde{n}+m+\tilde{m}$ local
maximum points involving
$q_1,\ldots,q_n$,  $q^p_{n+\tilde{n}+1},\ldots,q^p_{n+\tilde{n}+m}\in\Omega$,
and
$q_{n+1},\ldots,q_{n+\tilde{n}}$,
$q^p_{n+\tilde{n}+m+1},\ldots,q^p_{n+\tilde{n}+m+\tilde{m}}
\in\partial\Omega$. Moreover, $u_p$ has the following concentration property:
$$
pS(x)u^{p+1}_p\rightharpoonup
e\sum_{l\in J_1\cup J_2}d_l\delta_{q_l}+e\sum_{l\in J_3
\cup J_4}d_l\delta_{\tilde{q}_l}
\quad\text{as } p\to+\infty,
$$
where $\tilde{q}=(\tilde{q}_{n+\tilde{n}+1},\ldots,
\tilde{q}_{n+\tilde{n}+m+\tilde{m}})$ is a
global  minimum point of $\varphi^{\tilde{m}}_{m}$ in
$\Lambda^{\tilde{m}}_{m}(\delta)$
such that for $l\in J_3\cup J_4$,
$\operatorname{dist}(q^p_l,\,\tilde{q}_l)\to0$ as $p\to+\infty$.
Furthermore,
$$
u_p\to0\quad \text{uniformly in }
\overline{\Omega}\setminus
\cup_{l\in J_1\cup J_2}B_{\delta}(q_l)\cup
\cup_{l\in J_3\cup J_4}B_{\delta}(q^p_l),
$$
and  for the points $q_l$, $l\in J_1\cup J_2$, and $q^p_l$, $l\in J_3\cup J_4$,
$$
\sup_{x\in\overline{\Omega}\cap B_{\delta}(q_l)}u_p(x)\to\sqrt{e},\quad
\sup_{x\in\overline{\Omega} \cap B_{\delta}(q^p_l)}u_p(x)\to\sqrt{e},
$$
as $p\to+\infty$.
\end{theorem}


\begin{remark} \label{rmk1.3}\rm
The assumption  $\inf_{\overline{\Omega}}c>0$ guarantees the
existence of global minimum for the function $\varphi^{\tilde{m}}_{m}$
in $\Lambda^{\tilde{m}}_{m}(\delta)$, which  follows from properties of
the Green's function. The proof is similar to \cite[Lemma 6.1]{MW1}.
\end{remark}

\begin{remark} \label{rmk1.4}\rm
Assume that $\inf_{\overline{\Omega}}c>0$ and $\partial\Omega\setminus\Gamma_2$
has at least one circle, by Ljusternik-Schnirelman theory, we can find
another distinct solution satisfying Theorem \ref{thm1.2}.
The proof is similar to the one in \cite{DDM}.
\end{remark}

Note that  Theorem \ref{thm1.2} was partly proved  in \cite{MW1} only when $S\equiv 1$.
Moreover,
comparing to the  result of  \cite{MW1},  this theorem  provides a similar but
more complex concentration  phenomenon involving the presence of
mixed interior and boundary peak solutions to \eqref{a}.
Indeed,
Theorem \ref{thm1.2} implies  the existence of
solutions for \eqref{a} concentrating at points
$q_l$, $l\in J_1\cup J_2$, and $\tilde{q}_l$, $l\in J_3\cup J_4$.
Unlike  concentration set in \cite{MW1} only contains
no  source points in the domain and on the boundary,
our concentration set also contains  some  interior  source
points   $q_l$, $l\in J_1$, and  boundary source points   $q_l$,
$l\in J_2$.
This in return implies that the presence of  mixed interior and boundary
source points makes sure   that  some interior or boundary peak points of
 solutions of \eqref{a} always  locate at these source points.
For this reson, if we consider a very  simple  case  of  the H\'enon-type weight
defined in \eqref{a2}, where
\begin{equation}
S(x)=|x-0|^{2\alpha}\quad
\text{with $0\in\overline{\Omega}$ and $-1<\alpha\not\in\mathbb{N}\cup\{0\}$},
\end{equation}
then the corresponding problem \eqref{*} always admits a family of positive solutions
 with arbitrarily
many interior and boundary spikes  involving  the origin when $p$ tends to $+\infty$,
which implies the result in Theorem \ref{thm1.1} hold.
Besides,  we also point out the interesting result in \cite{D}
that  solutions for the Liouville equation
with the H\'enon-type weight only
concentrate at interior points different from the location
of the sources.

Finally, it is necessary to mention the analogy existing between our results
and those known for the Dirichlet problem in $\mathbb{R}^2$:
\begin{equation}\label{a5}
\begin{gathered}
-\Delta u=S(x)u^p\quad \text{in } \Omega,\\
u>0 \quad \text{in } \Omega,\\
u=0 \quad \text{on } \partial\Omega.
\end{gathered}
\end{equation}
Let us point out that  \eqref{a5} does not allow any
 solution with boundary spike-layer profile to exist (see \cite{GNN}),
which shows that  the Dirichlet boundary condition is far more rigid than
 the Neumann boundary condition. For  $S\equiv1$,
asymptotic behavior of least energy solutions of \eqref{a5}
is well understood after the works \cite{AG,EG,RW,RW1}: $pu^{p+1}$
approaches a Dirac mass at the harmonic center of $\Omega$  when $p$ tends to
infinity. Construction of solutions with this behavior has been achieved in
\cite{EMP1}, in which it is shown that for $S\equiv1$, problem \eqref{a5}
has solutions with $m$ interior spikes if $\Omega$ is not simply connected.
As for the case of the H\'enon-type weight
\begin{equation}\label{a6}
S(x)=c(x)\prod_{i=1}^n|x-q_i|^{2\alpha_i},
\end{equation}
where
$n\geq1$,
$q_1,\ldots,q_n\in\Omega$,
$-1<\alpha_1,\ldots,\alpha_n\not\in\mathbb{N}\cup\{0\}$
and $c: \Omega\to \mathbb{R}$  is a continuous function such that
$c(q_i)>0$ for all $i=1,\ldots,n$,
related constructions for problem \eqref{a5}
have also been performed  in \cite{CY2,EPW},
in which it is shown that under a $C^0$-stable critical
 point  assumption there exists a family of positive solutions
with exactly $n+m$ interior spikes
involving source points $q_1,\ldots,q_n$ as $p$ tends to
$+\infty$.

The general strategy for proving our main results  relies on a
Lyapunov-Schmidt reduction procedure, which has appeared in many of
the other results mentioned above,  as in \cite{DKM,EGP,EMP1,EPW,MW1}.
The sketch of this procedure is given as follows:
in Section 2 we  describe exactly the ansatz for the solution that we are
searching for.
Then we rewrite  problem \eqref{a} in terms of a linearized operator for which
a solvability theory, subject to suitable orthogonality conditions,
is performed  through solving a linearized  problem and an intermediate
nonlinear problem in Section 3. In Section 4 we reduce problem \eqref{a}
to finding critical points of a finite-dimensional function and give its
asymptotic expansion.
Finally, the proof of Theorem  \ref{thm1.2}  is contained in Section 5.

\section{Ansatz}

In this section we describe the  approximate solution
for  \eqref{a} and then we estimate the error of
such approximation in appropriate norms.

We first fix $n+\tilde{n}$
distinct source points $q_i$, $i\in J_1\cup J_2$,
and for $\delta>0$ sufficiently small but fixed we choose points
$q=(q_{n+\tilde{n}+1},\ldots,q_{n+\tilde{n}+m+\tilde{m}})
\in\Lambda_{m}^{\tilde{m}}(\delta)$.
Moreover, we set
\begin{equation}
\varepsilon_p=e^{-p/4},
\end{equation}
and consider  positive numbers $\mu_i$ such that
\begin{equation}
\delta<\mu_i<\delta^{-1} \quad \forall i\in\cup_{l=1}^4J_l.
\end{equation}
We  define the function
\begin{equation}\label{2.0}
u_{i}(x)=\log\frac{8(1+\alpha_i)^2\varepsilon_p^2\mu_i^2}
{[\varepsilon^2_p\mu_i^2+|x-q_i|^{2(1+\alpha_i)}]^2},
\end{equation}
and a correction term  as the solution of
\begin{equation}\label{2.1}
\begin{gathered}
-\Delta H_i+H_i=-u_i\quad\text{in }\Omega,\\
\frac{\partial H_i}{\partial \nu}=-\frac{\partial  u_i}{\partial \nu}
\quad \text{on }\partial\Omega.
\end{gathered}
\end{equation}

\begin{lemma} \label{lem2.1}
For any $0<\tau<1/2$ and for any $i\in\cup_{l=1}^4J_l$, then we have
\begin{equation}\label{2.6e}
H_i(x)=d_iH(x,q_i)+\frac{1}{2}p-\log8(1+\alpha_i)^2\mu_i^2+O(e^{-\tau\frac{p}{4}}),
\end{equation}
uniformly in $\overline{\Omega}$, where $H$ is the regular part of Green's
function defined by \eqref{f1}.
\end{lemma}

\begin{proof}
Note that, on the boundary, we have
$$
\frac{\partial H_i}{\partial \nu}=-\frac{\partial u_i}{\partial \nu}
=4(1+\alpha_i)|x-q_i|^{2\alpha_i}\frac{(x-q_i)\cdot\nu(x)}
{\varepsilon^2_p\mu_i^2+|x-q_i|^{2(1+\alpha_i)}}.
$$
Thus,
$$
\lim_{p\to\infty}\frac{\partial H_i}{\partial\nu}=4(1+\alpha_i)
\frac{(x-q_i)\cdot\nu(x)}
{|x-q_i|^2}\quad \forall x\in\partial\Omega\setminus\{q_i\}.
$$
On the other hand, by \eqref{f}-\eqref{f1}, the regular part of Green's
function $H(x,q_i)$ satisfies
\begin{equation}\label{2.11a}
\begin{gathered}
-\Delta H(x,q_i)+H(x,q_i)=\frac{4(1+\alpha_i)}{d_i}\log |x-q_i|\quad
\text{in } \Omega,\\
\frac{\partial H(x,q_i)}{\partial \nu}
=\frac{4(1+\alpha_i)}{d_i}\frac{(x-q_i)\cdot\nu(x)} {|x-q_i|^2}\quad
\text{on } \partial\Omega.
\end{gathered}
\end{equation}
So, if we set
$s_i(x)=H_i(x)-d_i H(x,q_i)-\frac12p+\log8(1+\alpha_i)^2\mu_i^2$,  we obtain
\begin{gather*}
-\Delta s_i+s_i=\log\frac{1}{|x-q_i|^{4(1+\alpha_i)}}-
\log\frac1{[\varepsilon_p^2\mu_i^2+|x-q_i|^{2(1+\alpha_i)}]^2}\quad
\text{in }\Omega,\\
\frac{\partial s_i}{\partial \nu}=\frac{\partial H_i}{\partial \nu}
-4(1+\alpha_i)\frac{(x-q_i)\cdot\nu(x)} {|x-q_i|^2} \quad
\text{on }\partial\Omega.
\end{gather*}
A direct computation shows that for any $\beta\in(1,+\infty)\cap(\frac2{1+\alpha_i},+\infty)$,
there exists a positive constant $C$ such that
\begin{gather*}
\big\|\frac{\partial H_i}{\partial \nu}-4(1+\alpha_i)\frac{(x-q_i)\cdot\nu(x)}
{|x-q_i|^2}\big\|_{L^\beta(\partial\Omega)}\leq Ce^{-\frac1{4\beta(1+\alpha_i)}p},
\\
\big\|\log\frac{1}{|x-q_i|^{4(1+\alpha_i)}}-
\log\frac1{[\varepsilon_p^2\mu_i^2+|x-q_i|^{2(1+\alpha_i)}]^2}
\big\|_{L^\beta(\Omega)}\leq Cpe^{-\frac1{2\beta(1+\alpha_i)}p}.
\end{gather*}
By $L^\beta$ theory
$$
\|s_{i}\|_{W^{1+s,\beta}(\Omega)}
\leq C(\|\Delta
s_i\|_{L^{\beta}(\Omega)}+\|\frac{\partial s_i}{\partial \nu}\|_{L^\beta(\partial\Omega)})
\leq Ce^{-\frac1{4\beta(1+\alpha_i)}p}
$$
for $0<s<1/\beta$. By  Morrey embedding we obtain
$$
\|s_i\|_{C^{\tilde{s}}(\overline{\Omega})}
\leq Ce^{-\frac1{4\beta(1+\alpha_i)}p}
$$
for $0<\tilde{s}<\frac12+\frac1\beta$.
This proves the result (with  $\tau=\frac1{\beta(1+\alpha_i)}$).
\end{proof}

We now define the first ansatz  as
$$
U_q(x)=\sum_{i=1}^{n+\tilde{n}+m+\tilde{m}}\,
\frac1{\gamma \mu_i^{\frac2{p-1}}
c_i(q_i)^{\frac1{p-1}}} [u_i(x)+H_i(x)],
$$
where
$$
\gamma=p^{\frac{p}{p-1}}\varepsilon_p^{\frac{2}{p-1}}=
p^{\frac{p}{p-1}}e^{-\frac{p}{2(p-1)}}.
$$
We shall show later that $U_q(x)$ is a good approximation for a solution
of problem \eqref{a} in a region far away from the points $q_i$,
but  unfortunately it is  not good enough for our construction
close to these points.
Thus, we need to further adjust this ansatz
by adding two other terms to the expansion of the solution.
To do this, we set
\begin{gather}\label{2.0a}
U^i(x)=\log\frac{8(1+\alpha_i)^2}{[1+|x|^{2(1+\alpha_i)}]^2}, \\
\label{2.0b}
\rho_i=\varepsilon_p^{\frac1{1+\alpha_i}},\quad
v_i=\mu_i^{\frac1{1+\alpha_i}},\quad
z_i=\frac{1}{v_i\rho_i}(x-q_i).
\end{gather}
Define  the functions $\omega^{ji}$, $j=0,1$, as  radial solutions of
\begin{equation}\label{2.3}
\Delta \omega^{ji}+|x|^{2\alpha_i}e^{U^i}\omega^{ji}
=|x|^{2\alpha_i}f^{ji}\quad\text{in }\mathbb{R}^2,
\end{equation}
and define
\begin{gather}\label{2.3a}
f^{0i}(x)=\frac12 e^{U^i}(U^i)^2, \\
\label{2.4}
f^{1i}(x)=e^{U^i}\big\{\omega^{0i}U^i-\frac12(\omega^{0i})^2-\frac13(U^i)^
3-\frac18(U^i)^4+\frac12\omega^{0i}(U^i)^2\big\},
\end{gather}
with the property that
\begin{equation}\label{2.5a}
\omega^{ji}=C_{ji}\log|x|+O(\frac1{|x|^{1+\alpha_i}})\quad
\text{as } |x|\to+\infty,
\end{equation}
for some constant $C_{ji}$, which can be  explicitly computed through
the formula
$$
C_{ji}=\int_0^{+\infty}r^{2\alpha_i+1}\frac{r^{2(1+\alpha_i)}-1}
{r^{2(1+\alpha_i)}+1}f^{ji}(r)dr.
$$
The existence of $\omega^{0i}$ and $\omega^{1i}$ with such properties
can be obtained as in \cite{CY2,EMP1,EPW}.
In particular,
\begin{equation}\label{2.5c}
\begin{aligned}
\omega^{0i}(x)
&=\frac12(U^i)^2(x)+6\log[1+|x|^{2(1+\alpha_i)}]
+\frac{2\log8(1+\alpha_i)^2-10}{|x|^{2(1+\alpha_i)}+1}\\
&\quad+\frac{|x|^{2(1+\alpha_i)}-1}{|x|^{2(1+\alpha_i)}+1}
\Big\{2\log^2[1+|x|^{2(1+\alpha_i)}]-\frac12\log^28(1+\alpha_i)^2 \\
&\quad +4\int_{|x|^{2(1+\alpha_i)}}^{+\infty}\frac{ds}{s+1}
\log\frac{s+1}{s}
-8(1+\alpha_i)\log|x|\log[1+|x|^{2(1+\alpha_i)}]\Big\}.
\end{aligned}
\end{equation}
Moreover, it is easy to compute the value
\begin{equation}\label{2.5b}
C_{0i}=12(1+\alpha_i)-4(1+\alpha_i)\log8(1+\alpha_i)^2.
\end{equation}
Now, we define the functions
\begin{equation}\label{2.4a}
\omega_{ji}(x)=\omega^{ji}\big(\frac{x-q_i}{v_i\rho_i}\big)\quad
\text{for }j=0,1,
\end{equation}
and its new correction term as the solution of
\begin{equation}\label{2.2}
\begin{gathered}
-\Delta H_{ji}+H_{ji}=-\omega_{ji}\quad \text{in }\Omega,\\
\frac{\partial H_{ji}}{\partial \nu}
=-\frac{\partial \omega_{ji}}{\partial \nu}
\quad \text{on } \partial\Omega.
\end{gathered}
\end{equation}

\begin{lemma} \label{lem2.2}
For any $0<\tau<\frac12$ and for any $i\in\cup_{l=1}^4J_l$, $j=0,1$, we have
\begin{equation}\label{2.6g}
H_{ji}(x)=-\frac{d_iC_{ji}}{4(1+\alpha_i)}H(x,q_i)
+\frac{C_{ji}}{1+\alpha_i}\log\mu_i-\frac{pC_{ji}}{4(1+\alpha_i)}
+O(e^{-\tau\frac{p}{4}}),
\end{equation}
uniformly in $\overline{\Omega}$, where $H$ is the regular part of Green's
function defined by \eqref{f1}.
\end{lemma}

\begin{proof}
The proof is the same as Lemma \ref{lem2.1}.
 First, on the boundary, we have
$$
\lim_{p\to\infty}\frac{\partial H_{ji}}{\partial\nu}
=-C_{ji}\frac{(x-q_i)\cdot\nu(x)}
{|x-q_i|^2}\quad \forall x\in\partial\Omega\setminus\{q_i\}.
$$
Define
\[
\tilde{s}_i(x)=H_{ji}(x)+\frac{d_iC_{ji}}{4(1+\alpha_i)}H(x,q_i)
-\frac{C_{ji}}{1+\alpha_i}\log\mu_i+\frac{pC_{ji}}{4(1+\alpha_i)},
\]
 by using \eqref{2.11a},  we  get
\begin{gather*}
-\Delta \tilde{s}_i+\tilde{s}_i=-\omega_{ji}+C_{ji}\log|x-q_i|
 -\frac{C_{ji}}{1+\alpha_i}\log\mu_i+\frac{pC_{ji}}{4(1+\alpha_i)}
\quad \text{in } \Omega,\\
\frac{\partial \tilde{s}_i}{\partial \nu}
=\frac{\partial H_{ji}}{\partial \nu}+C_{ji}\frac{(x-q_i)\cdot\nu(x)}
{|x-q_i|^2} \quad \text{on } \partial\Omega.
\end{gather*}
From \eqref{2.5a} and \eqref{2.4a}, we can get that for any
$\beta\in(1,+\infty)\cap(\frac2{1+\alpha_i},+\infty)$,
there exists a positive constant $C$ such that
\begin{gather*}
\big\|\frac{\partial H_{ji}}{\partial \nu}+C_{ji}\frac{(x-q_i)\cdot\nu(x)}
{|x-q_i|^2}\big\|_{L^\beta(\partial\Omega)}\leq Ce^{-\frac1{4\beta(1+\alpha_i)}p},
\\
\big\|-\omega_{ji}+C_{ji}\log|x-q_i|-\frac{C_{ji}}{1+\alpha_i}
\log\mu_i+\frac{pC_{ji}}{4(1+\alpha_i)}
\big\|_{L^\beta(\Omega)}\leq Ce^{-\frac1{2\beta(1+\alpha_i)}p}.
\end{gather*}
This, and the same procedure as the proof of Lemma \ref{lem2.1},
easily implies that  \eqref{2.6g} also holds.
\end{proof}

Now, we define the  first  approximation of the solution  for  problem \eqref{a} as
\begin{equation}\label{2.6}
U_q(x)=\sum_{i=1}^{n+\tilde{n}+m+\tilde{m}}
\frac1{\gamma\,\mu_i^{\frac2{p-1}}
c_i(q_i)^{\frac1{p-1}}}
\big[u_i+H_i+\frac1p(\omega_{0i}+H_{0i})+\frac1{p^2}(\omega_{1i}+H_{1i})\big](x).
\end{equation}
From Lemmas \ref{lem2.1}--\ref{lem2.2},  away from the points $q_i$, $i\in\cup_{l=1}^4J_l$,
one has
\begin{equation}\label{2.6a}
U_q(x)=\sum_{i=1}^{n+\tilde{n}+m+\tilde{m}}
\frac{d_iG(x,q_i)}{\gamma\,\mu_i^{\frac2{p-1}}
c_i(q_i)^{\frac1{p-1}}}\big[1
-\frac{C_{0i}}{4p(1+\alpha_i)}-\frac{C_{1i}}{4p^2(1+\alpha_i)}
+O(\varepsilon_p^\tau)\big].
\end{equation}

Consider now the change of variables
$$
v(y)=\varepsilon_p^{\frac2{p-1}}u(\varepsilon_p y)
\quad\text{for } y\in\Omega_{\varepsilon},
$$
where $\Omega_{\varepsilon}=\frac1{\varepsilon_p}\Omega$,
then problem \eqref{a} reduces to
\begin{equation}\label{2.13}
\begin{gathered}
-\Delta v+\varepsilon_p^2v=S(\varepsilon_p y)v^p\quad
\text{in } \Omega_{\varepsilon},\\
 v>0 \quad \text{in } \Omega_{\varepsilon},\\
\frac{\partial v}{\partial\nu}=0 \quad
\text{on }\partial\Omega_{\varepsilon}.
\end{gathered}
\end{equation}
Let us define the first approximation solution of \eqref{2.13} as
\begin{equation}\label{2.13a}
V_q(y)=\varepsilon_p^{\frac2{p-1}}U_q(\varepsilon_p y),
\end{equation}
where $U_q$ is defined by \eqref{2.6}. For $|\varepsilon_py-q_i|<\delta$ with
$\delta$ sufficiently small
but fixed, by using Lemmas \ref{lem2.1}--\ref{lem2.2} and \eqref{2.6a}, we have
\begin{align*} %\label{2.7b}
&V_q(y)\\
&= \frac1{p^{\frac{p}{p-1}}\mu_i^{\frac2{p-1}}
c_i(q_i)^{\frac1{p-1}}}[u_i+H_i+\frac1p(\omega_{0i}+H_{0i})
+\frac1{p^2}(\omega_{1i}+H_{1i})] \\
&\quad +\sum_{j\neq i} \frac1{p^{\frac{p}{p-1}}\mu_j^{\frac2{p-1}}
c_j(q_j)^{\frac1{p-1}}}[u_j+H_j+\frac1p(\omega_{0j}+H_{0j})
+\frac1{p^2}(\omega_{1j}+H_{1j})] \\
&=\frac1{p^{\frac{p}{p-1}}\mu_i^{\frac2{p-1}}
c_i(q_i)^{\frac1{p-1}}}\Big\{
\big[U^i(\frac{x-q_i}{v_i\rho_i})+\frac12p-\log\mu_i^2\big]+
\big[d_iH(x,q_i)+\frac{1}{2}p \\
&\quad -\log8(1+\alpha_i)^2\mu_i^2\big]
 +\frac1p\big[\omega_{0i}-\frac{d_iC_{0i}}{4(1+\alpha_i)}H(x,q_i)
+\frac{C_{0i}}{1+\alpha_i}\log\mu_i-\frac{pC_{0i}}{4(1+\alpha_i)}\big] \\
&\quad  +\frac1{p^2}\big[\omega_{1i}-\frac{d_iC_{1i}}{4(1+\alpha_i)}H(x,q_i)
+\frac{C_{1i}}{1+\alpha_i}\log\mu_i-\frac{pC_{1i}}{4(1+\alpha_i)}\big]
+O(\varepsilon_p^\tau)\Big\}\\
&\quad +\sum_{j\neq i}
\frac{d_jG(x,q_j)}{p^{\frac{p}{p-1}}\mu_j^{\frac2{p-1}}c_j(q_j)^{\frac1{p-1}}}
\big[1-\frac{C_{0j}}{4p(1+\alpha_j)}-\frac{C_{1j}}{4p^2(1+\alpha_j)}
+O(\varepsilon_p^\tau)\big] \\
&=\frac1{p^{\frac{p}{p-1}}\mu_i^{\frac2{p-1}}c_i(q_i)^{\frac1{p-1}}}
\Big\{p+U^i(\frac{x-q_i}{v_i\rho_i})+\frac{1}p\omega_{0i}
 +\frac{1}{p^2}\omega_{1i}+O(|x-q_i|)+O(\varepsilon^\tau_p)  \\
&\quad -\log8(1+\alpha_i)^2\mu_i^4+d_i
\big[1-\frac{C_{0i}}{4p(1+\alpha_i)}
 -\frac{C_{1i}}{4p^2(1+\alpha_i)}\big]H(q_i,q_i) \\
&\quad + \frac{1}{p(1+\alpha_i)}\big(C_{0i}+\frac{1}pC_{1i}\big)
\big(\log\mu_i-\frac14p\big) \\
&\quad +\sum_{j\neq i}\big[\frac{\mu_i^2c_i(q_i)}{\mu_j^2c_j(q_j)}
\big]^{\frac1{p-1}}d_j
\big[1-\frac{C_{0j}}{4p(1+\alpha_j)}-\frac{C_{1j}}{4p^2(1+\alpha_j)}\big]
G(q_i,q_j)\Big\}.
\end{align*}
We now choose the parameters $\mu_i$: we assume  they are defined by the relation
\begin{align*}\label{2.6b}
\log8(1+\alpha_i)^2\mu_i^4
&=d_i \big[1-\frac{C_{0i}}{4p(1+\alpha_i)}-\frac{C_{1i}}{4p^2(1+\alpha_i)}\big]
 H(q_i,q_i) \\
&\quad + \frac{1}{p(1+\alpha_i)}\big(C_{0i}+\frac{1}pC_{1i}\big)
\big(\log\mu_i-\frac14p\big) \\
&\quad +\sum_{j\neq i}\big[\frac{\mu_i^2c_i(q_i)}{\mu_j^2c_j(q_j)}
 \big]^{\frac1{p-1}}d_j
\big[1-\frac{C_{0j}}{4p(1+\alpha_j)}-\frac{C_{1j}}{4p^2(1+\alpha_j)}\big]G(q_i,q_j).
\end{align*}
Taking into account the explicit expression \eqref{2.5b}  of the constant
$C_{0i}$, we observe that $\mu_i$ bifurcates, as $p$ tends to $+\infty$,
from the value
\begin{equation}\label{2.6bbc}
\bar{\mu}_i=e^{-\frac34}e^{\frac14[d_iH(q_i,q_i)
+\sum_{j\neq i}d_jG(q_j,q_i)]},
\end{equation}
solution of the equation
\begin{equation}\label{2.6c}
\log8(1+\alpha_i)^2\mu_i^4=d_iH(q_i,q_i)
-\frac{C_{0i}}{4(1+\alpha_i)}+\sum_{j\neq i}d_jG(q_i,q_j).
\end{equation}
Thus, $\mu_i$ is a perturbation of order $\frac1p$ of the value $\bar{\mu}_i$,
namely
\begin{equation}\label{2.6bb}
\mu_i=e^{-\frac34}e^{\frac14[d_iH(q_i,q_i)
+\sum_{j\neq i}d_jG(q_j,q_i)]}\left(1+O(\frac1p)\right).
\end{equation}
From this choice of the parameters $\mu_i$, we deduce that for
$|\varepsilon_py-q_i|<\delta$,
\begin{equation}\label{2.7c}
V_q(y)
=\frac1{p^{\frac{p}{p-1}}\mu_i^{\frac2{p-1}}c_i(q_i)^{\frac1{p-1}}}\big[
p+U^i(z_i)+\frac{1}p\omega^{0i}(z_i)+\frac{1}{p^2}\omega^{1i}(z_i)
+\theta(y)\big],
\end{equation}
with
$$
z_i=\frac{1}{v_i\rho_i}(\varepsilon_py-q_i),\quad
\theta(y)=O(\rho_i|z_i|)+O(\varepsilon^\tau_p).
$$

In the rest of this paper, we will seek solutions  of  problem
\eqref{2.13} in the form
$v=V_q+\phi$, where $\phi$ will represent a lower order correction.
In terms of $\phi$, problem \eqref{2.13} becomes
\begin{equation}\label{2.23}
\begin{gathered}
L(\phi):=-\Delta
\phi+\varepsilon_p^2\phi-W_q\phi=R_q+N(\phi)\quad
\text{in }\Omega_{\varepsilon},\\
\frac{\partial \phi}{\partial\nu}=0
\quad \text{on }\partial\Omega_{\varepsilon},
\end{gathered}
\end{equation}
where
\begin{equation}\label{2.13b}
W_q=pS(\varepsilon_p y)V_q^{p-1},
\end{equation}
$R_q$ is the ``error term''
\begin{equation}\label{2.13bb}
R_q=\Delta V_q-\varepsilon_p^2V_q+S(\varepsilon_p y)V_q^p,
\end{equation}
and $N(\phi)$ stands for  the ``nonlinear term''
\begin{equation}\label{2.24}
N(\phi)=S(\varepsilon_p y) [(V_q+\phi)^p-V^p_q-pV_q^{p-1}\phi].
\end{equation}
The main step in solving problem \eqref{2.23} for small $\phi$ is, under
a suitable choice of the points $q_i$, that of a solvability theory
for the linear operator $L$. In developing this theory,
we introduce a    weighted $L^\infty$-space
$$
\mathcal {C}_{*}=\{h\in L^{\infty}(\Omega_\varepsilon):
\|h\|_{*}<+\infty\},
$$
with the norm
\begin{equation}\label{3.2a}
\|h\|_{*}=\sup_{y\in\overline{\Omega}_{\varepsilon}}
\frac{|h(y)|}{\varepsilon_p^2+\sum_{\alpha_i<0,\,i\in
J_1\cup J_2}\frac{(\frac{\varepsilon_p}{v_i\rho_i})^2
|z_i|^{2\alpha_i}}{(1+|z_i|)^{4+2\alpha+2\alpha_i}}+\sum_{\alpha_i\geq
0,\,i\in\cup_{l=1}^{4}J_{l}}
\frac{(\frac{\varepsilon_p}{v_i\rho_i})^2}{(1+|z_i|)^{4+2\alpha}}}\,,
\end{equation}
where we fix $-1<\alpha<\alpha_0$ with
$\alpha_0=\min\{\alpha_i: i\in\cup_{l=1}^4J_l\}$. With respect to the
norm \eqref{3.2a}, the error term $R_q$ defined in \eqref{2.13bb}
can be estimated in the following way.

\begin{lemma} \label{lem2.3}
For $\delta>0$  sufficiently small but fixed,
there exist $C$, $D_0>0$ and $p_0>1$ such that
\begin{gather}\label{2.22}
\|R_q\|_*\leq C/p^4, \\
\label{2.19}
W_q(y)\leq D_0\sum_{i=1}^{n+\tilde{n}+m+\tilde{m}}
(\frac{\varepsilon_p}{v_i\rho_i})^2|z_i|^{2\alpha_i}e^{U^i(z_i)},
\end{gather}
for any $q\in\Lambda_{m}^{\tilde{m}}(\delta)$
and $p\geq p_0$. Furthermore,
\begin{equation}\label{2.18c}
W_q(y)=(\frac{\varepsilon_p}{v_i\rho_i})^2|z_i|^{2\alpha_i}e^{U^i(z_i)}
\big[1+\frac{\omega^{0i}-U^i-\frac12(U^i)^2}p
+O(\frac{\log^4(2+|z_i|)}{p^2})\big],
\end{equation}
for any $|z_i|\leq\delta(v_i\rho_i)^{-1/2}$, where
$z_i=\frac{\varepsilon_py-q_i}{v_i\rho_i}$.
\end{lemma}

\begin{proof}
Observe that by  \eqref{2.1},
\begin{gather*}
-\Delta (u_i+H_i)+\varepsilon_p^2(u_i+H_i)
=(\frac{\varepsilon_p}{v_i\rho_i})^2|z_i|^{2\alpha_i}e^{U^i(z_i)}
\quad \text{in } \Omega_\varepsilon,\\
\frac{\partial}{\partial \nu}(u_i+H_i)=0 \quad \text{on } \partial\Omega_\varepsilon,
\end{gather*}
and by \eqref{2.3}  and  \eqref{2.2}, for $j=0,1$,
\begin{gather*}
-\Delta(\omega_{ji}+
H_{ji})+\varepsilon_p^2(\omega_{ji}+H_{ji})
=(\frac{\varepsilon_p}{v_i\rho_i})^2|z_i|^{2\alpha_i}
(e^{U^i}\omega^{ji}-f^{ji})(z_i)\quad
\text{in }\Omega_\varepsilon,\\
\frac{\partial}{\partial \nu}(\omega_{ji}+H_{ji})=0\quad
\text{on }\partial\Omega_\varepsilon,
\end{gather*}
which combined with the definition of $V_q$  in  \eqref{2.13a}
can deduce directly that
\begin{equation}\label{2.13c}
\begin{aligned}
&-\Delta V_q+\varepsilon_p^2V_q\\
&=\sum_{i=1}^{n+\tilde{n}+m+\tilde{m}}
\frac{(\frac{\varepsilon_p}{v_i\rho_i})^2|z_i|^{2\alpha_i}}
{p^{\frac p{p-1}}\mu_i^{\frac2{p-1}}
c_i(q_i)^{\frac1{p-1}}}
\big[e^{U^i}+\frac{e^{U^i}\omega^{0i}-f^{0i}}p
+\frac{e^{U^i}\omega^{1i}-f^{1i}}{p^2}\big](z_i).
\end{aligned}
\end{equation}
From the definition \eqref{2.0a} of $U^i$ and the asymptotic behavior \eqref{2.5a}
of $\omega^{ji}$, $j=0,1$, we obtain that in a region far away from the points
$q_i$, namely for $|x-q_i|>\delta$; i.e.
$|z_i|>\delta(v_i\rho_i)^{-1}$ for all $i$,
$$
U^i(z_i)=-p+O(1),\quad \omega^{ji}(z_i)=\frac{C_{ji}}{4(1+\alpha_i)}p+O(1),
$$
and so
\begin{equation}\label{2.13d}
\big[e^{U^i}+\frac{e^{U^i}\omega^{0i}-f^{0i}}p
+\frac{e^{U^i}\omega^{1i}-f^{1i}}{p^2}\big](z_i)=O(p^2e^{-p}).
\end{equation}
This, together with \eqref{2.6a} and \eqref{2.13a}  imply
\begin{equation}\label{2.21}
R_q=O(pe^{-p})+O(p^{-p-1}).
\end{equation}
Let us now fix the index $i$ and the region $|z_i|\leq\delta(v_i\rho_i)^{-1/2}$.
 From \eqref{2.7c} we obtain
\begin{equation}\label{2.7a}
\begin{aligned}
S(\varepsilon_p y)V_q^p
&=\frac{(\frac{\varepsilon_p}{v_i\rho_i})^2|z_i|^{2\alpha_i}}
{p^{\frac{p}{p-1}}\mu_i^{\frac{2}{p-1}}
c_i(q_i)^{\frac{1}{p-1}}}(1+O(\rho_i|z_i|))
\Big[1+\frac{U^i(z_i)}{p}\\
&\quad +\frac{\omega^{0i}(z_i)}{p^2}
+\frac{\omega^{1i}(z_i)}{p^3}
+\frac{\theta(y)}{p}\Big]^p.
\end{aligned}
\end{equation}
By the Taylor expansions of the exponential and logarithmic function, we have
for $|z_i|\leq\delta(v_i\rho_i)^{-1/2}$,
\begin{equation}\label{2.7f}
\begin{aligned}
&\Big(1+\frac{a}p+\frac{b}{p^2}+\frac{c}{p^3}\Big)^p\\
&=e^a\big[1+\frac1p\big(b-\frac{a^2}2\big)+\frac1{p^2}\big(c-ab+\frac{a^3}3
+\frac{b^2}2+\frac{a^4}8-\frac{a^2b}2\big) \\
&\quad +O(\frac{\log^6(|z_i|+1)}{p^3})\big],
\end{aligned}
\end{equation}
provided $-5(1+\alpha_i)\log(|z_i|+2)\leq a(z_i)\leq C$ and
$|b(z_i)|+|c(z_i)|\leq C\log(|z_i|+2)$.
Thus, for  $|z_i|\leq\delta(v_i\rho_i)^{-1/2}$,
\begin{equation}\label{2.7h}
\begin{aligned}
S(\varepsilon_p y)V_q^p
&=\frac{(\frac{\varepsilon_p}{v_i\rho_i})^2
|z_i|^{2\alpha_i}}{p^{\frac p{p-1}}\mu_i^{\frac2{p-1}}
c_i(q_i)^{\frac1{p-1}}}\big[e^{U^i}+\frac{e^{U^i}\omega^{0i}-f^{0i}}p
+\frac{e^{U^i}\omega^{1i}-f^{1i}}{p^2}\big](z_i)\\
&\quad + (\frac{\varepsilon_p}{v_i\rho_i})^2|z_i|^{2\alpha_i}e^{U^i(z_i)}
O\big(\frac{\log^6(|z_i|+2)}{p^4}
+\varepsilon^\tau_p+p^2\rho_i|z_i|\big).
\end{aligned}
\end{equation}
Joining together \eqref{2.13c}, \eqref{2.13d} and \eqref{2.7h},
in this region  we obtain
\begin{equation}\label{2.21b}
R_q=(\frac{\varepsilon_p}{v_i\rho_i})^2|z_i|^{2\alpha_i}e^{U^i(z_i)}
O(\frac{\log^6(|z_i|+2)}{p^4}
+\varepsilon^\tau_p+p^2\rho_i|z_i|)+O(pe^{-p}).
\end{equation}
On the other hand,  if
$\delta(v_i\rho_i)^{-1/2}\leq|z_i|\leq\delta(v_i\rho_i)^{-1}$, we have
\begin{equation}\label{2.17a}
-\Delta V_q+\varepsilon_p^2V_q
=O(p(\frac{\varepsilon_p}{v_i\rho_i})^2|z_i|^{2\alpha_i}e^{U^i(z_i)})+O(pe^{-p}),
\end{equation}
and by \eqref{2.7a},
\begin{equation}\label{2.7e}
S(\varepsilon_p y)V_q^p=O(\frac1p(\frac{\varepsilon_p}{v_i\rho_i})^2|z_i|^{2\alpha_i}
e^{U^i(z_i)}),
\end{equation}
since $(1+\frac{s}p)^s\leq e^s$. Thus, in this region
\begin{equation}\label{2.21a}
R_q=O(p(\frac{\varepsilon_p}{v_i\rho_i})^2|z_i|^{2\alpha_i}e^{U^i(z_i)})
+O(pe^{-p}).
\end{equation}
So,  estimate \eqref{2.22} can be easily derived from
\eqref{2.21}, \eqref{2.21b} and \eqref{2.21a}.


Finally, to prove the estimate over $W_q(y)=pS(\varepsilon_p y)V_q^{p-1}$,
we first notice a slight modification of formula \eqref{2.7f}
$$
\Big(1+\frac{a}p+\frac{b}{p^2}+\frac{c}{p^3}\Big)^{p-1}
=e^a\big[1+\frac1p\big(b-a-\frac{a^2}2\big)+
+O(\frac{\log^4(|z_i|+2)}{p^2})\big].
$$
Thus, for $|z_i|\leq\delta(v_i\rho_i)^{-1/2}$, by \eqref{2.7c},
\begin{align*}
W_q(y)
&=pS(\varepsilon_p y)V_q^{p-1}\\
&=\frac{c_i(\varepsilon_p y)|\varepsilon_p y-q_i|^{2\alpha_i}}{\mu_i^2c_i(q_i)}
\big[1+\frac{U^i}p+\frac{\omega^{0i}}{p^2}
 +\frac{\omega^{1i}}{p^3}+O(\frac{\rho_i|z_i|+\varepsilon^\tau_p}{p})\big]^{p-1}\\
&=(\frac{\varepsilon_p}{v_i\rho_i})^2|z_i|^{2\alpha_i}e^{U^i(z_i)}
\big[1+\frac{\omega^{0i}-U^i-\frac12(U^i)^2}p
+O(\frac{\log^4(2+|z_i|)}{p^2})\big].
\end{align*}
In addition, if $|z_i|\geq\delta(v_i\rho_i)^{-1}$ for
all $i$, we obtain that $W_q(y)=O(p^{1-p})$, and if
$\delta(v_i\rho_i)^{-1/2}<|z_i|<\delta(v_i\rho_i)^{-1}$,
$W_q(y)=O((\frac{\varepsilon_p}{v_i\rho_i})^2|z_i|^{2\alpha_i}e^{U^i(z_i)})$,
which completes the proof.
\end{proof}

\begin{remark} \label{rmk2.4} \rm
As for $W_q$, let us point out that if $|z_i|\leq\delta(v_i\rho_i)^{-1}$
for some $i$,
$$
pS(\varepsilon_p y)\Big(V_q+O(\frac1{p^3})\Big)^{p-2}
=O\Big((\frac{\varepsilon_p}{v_i\rho_i})^2|z_i|^{2\alpha_i}e^{U^i(z_i)}\Big).
$$
Since this estimate is true if  $|z_i|>\delta(v_i\rho_i)^{-1}$ for all
 $i\in\cup_{l=1}^4J_l$, we have
\begin{equation}\label{2.21e}
pS(\varepsilon_p y)\Big(V_q+O(\frac1{p^3})\Big)^{p-2}
\leq C\sum_{i=1}^{n+\tilde{n}+m+\tilde{m}}
(\frac{\varepsilon_p}{v_i\rho_i})^2|z_i|^{2\alpha_i}e^{U^i(z_i)}.
\end{equation}
\end{remark}

\section{The linearized problem and the nonlinear problem}

In this section we shall study first the following linear problem:
given $h$ of class $\mathcal {C}_{*}$ and points
$q
\in\Lambda_{m}^{\tilde{m}}(\delta)$, we find a function $\phi$, scalars
$c_{ij},\,i\in J_3$, $j=1,2$, and $c_{i1},\,i\in J_4$,
such that
\begin{equation}\label{3.3}
\begin{gathered}
L(\phi)=h+\sum_{i\in J_3\cup J_4}c_{i1}\chi_i\,Z_{i1}
+\sum_{i\in J_3}c_{i2}\chi_i\,Z_{i2}\quad \text{in }\Omega_{\varepsilon},\\
\frac{\partial\phi}{\partial\nu}=0\quad \text{on } \partial\Omega_{\varepsilon},\\
\int_{\Omega_{\varepsilon}}\chi_i Z_{ij}\phi=0\quad \forall i\in J_3,\;
j=1,2;\; i\in J_4,\; j=1,
\end{gathered}
\end{equation}
where $\chi_i$ and $Z_{ij}$ are defined as follows.
\begin{gather*}
L_i(\phi)=\Delta\phi+\frac{8(1+\alpha_i)^2|z|^{2\alpha_i}}{[1+|z|^{2(1+\alpha_i)}
]^2}\phi \quad \forall i\in\cup_{l=1}^4J_l,\quad
z_{i1}=\frac{4\operatorname{Re}(z)}{|z|^2+1} \quad \forall i\in J_3\cup J_4,\\
z_{i0}=\frac1{\mu_i}\frac{|z|^{2(1+\alpha_i)}-1}{|z|^{2(1+\alpha_i)}+1}\quad
\forall i\in\cup_{l=1}^4J_l\quad
z_{i2}=\frac{4\operatorname{Im}(z)}{|z|^2+1} \quad \forall i\in J_3\cup J_4.
\end{gather*}
It is well known that any bounded
solution to $L_i(\phi)=0$ in $\mathbb{R}^2$ is
 a linear combination of $z_{i0}$, $z_{i1}$ and $z_{i2}$ for
 $i\in J_3\cup J_4$ (see \cite{BP,CL5}), or
proportional to $z_{i0}$ for $i\in J_1\cup J_2$ (see \cite{CY1,E,EPW}).
Then  for  $i\in J_2\cup J_4$,
any bounded solution to $L_i(\phi)=0$ in
$\mathbb{R}_+^2$ and $\frac{\partial}{\partial z_2}\phi(z_1,0)=0$ on
$\partial\mathbb{R}_+^2$
is a linear combination of $z_{i0}$ and $z_{i1}$ if $i\in J_4$,
or proportional to $z_{i0}$ if $i\in J_2$.

For each point $q_i\in\partial\Omega$ with $i\in J_2\cup J_4$, we  have to strengthen
the boundary. Let us assume that $q_i=0$ and the unit outward
normal at $q_i$ is $(0,-1)$. Let $G(x_1)$ be the defining function for
the boundary $\partial\Omega$ in a neighborhood $B_\delta(q_i)$ of $q_i$,
that is, $\Omega\cap B_\delta(q_i)=\{(x_1,x_2)\in B_\delta(q_i): x_2>G(x_1)\}$.
Then let $F_i: B_\delta(q_i)\cap\overline{\Omega}\to \mathbb{R}^2$
be defined by $F_i=(F_{i1}, F_{i2})$, where
$$
F_{i1}=x_1+\frac{x_2-G(x_1)}{1+|G'(x_1)|^2}G'(x_1) \quad\text{and} \quad
F_{i2}=x_2-G(x_1).
$$
We consider
$\tilde{z}_i=F_i^\varepsilon(y)=\frac{1}{v_i\rho_i}F_i(\varepsilon_p y)$
and its inverse
$y=\tilde{F}^\varepsilon_i(\tilde{z}_i)
=\frac1{\varepsilon_p}F_i^{-1}(v_i\rho_i\tilde{z}_i)$. Set
$$
\tilde{z}_i(y):=\begin{cases}
z_i(y) & \forall i\in J_1\cup J_3,\\
F_i^\varepsilon(y) &\forall i\in J_2\cup J_4.
\end{cases}
$$
Furthermore, set
\begin{gather*}
Z_{i0}(y):= z_{i0}(\tilde{z}_i)\quad \forall i\in\cup_{l=1}^4J_l,\quad
Z_{i1}(y):= z_{i1}(\tilde{z}_i)\quad \forall i\in J_3\cup J_4,\\
Z_{i2}(y):=z_{i2}(\tilde{z}_i)\quad \forall i\in J_3,\quad
\chi_i(y):=\chi(|\tilde{z}_i|)\quad \forall i\in\cup_{l=1}^4J_l,
\end{gather*}
where $\chi(r)$ is a smooth, non-increasing cut-off function  such
that for a large but fixed number $R_0>0$,  $\chi(r)=1$ if $r\leq
R_0$,  and $\chi(r)=0$ if $r\geq R_0+1$. It is important to note that
$F_i$, $i\in J_2\cup J_4$,
preserves the  Neumann boundary condition and
\begin{equation}\label{3.2b}
\Delta_yZ_{i0}+W_{i0}Z_{i0}=\begin{cases}
0 & \forall \,i\in J_1\cup J_3,\\
O(\frac{\varepsilon_p^2}{v_i\rho_i}\frac{|z_i|^{2\alpha_i}}{(1+|z_i|)^{3+4\alpha_i}})
& \forall i\in J_2\cup J_4,
\end{cases}
\end{equation}
where
$$
W_{i0}:=\big(\frac{\varepsilon_p}{v_i\rho_i}\big)^2
\frac{8(1+\alpha_i)^2|z_i|^{2\alpha_i}}
{[1+|z_i|^{2(1+\alpha_i)}]^2}.
$$
The main result of this section is  the  following:

\begin{proposition} \label{prop3.1}
There exist  $C>0$  and $p_0>1$ such
that for any  $p\geq p_0$,   $h\in\mathcal {C}_{*}$ and
 $q\in\Lambda_{m}^{\tilde{m}}(\delta)$,
there exists a unique solution
$\phi\in L^{\infty}(\Omega_{\varepsilon})$,  scalars
$c_{ij},\,i\in J_3$, $j=1,2$, and $c_{i1},\,i\in J_4$, to
\eqref{3.3}. Moreover,  such solution satisfies
\begin{equation}\label{3.5}
\|\phi\|_{\infty}\leq Cp\|h\|_{*}.
\end{equation}
\end{proposition}

The proof will be divided into a series of lemmas which we state and prove next.


\begin{lemma} \label{lem3.2}
 For $p$ large enough, there exist  $R_1>0$, and
$$
\psi: \overline{\Omega}_{\varepsilon}\setminus
\cup_{i=1}^{n+\tilde{n}+m+\tilde{m}}B_{i,R_1}\,\,\longmapsto\,\mathbb{R}
$$
positive  and
uniformly bounded so that
\begin{equation}\label{3.7a}
\begin{gathered}
L(\psi)\geq\sum_{i\in\cup_{l=1}^{4}J_l}
(\frac{\varepsilon_p}{v_i\rho_i})^2\frac{1}{|z_i|^{4+2\alpha}}+\varepsilon_p^2
\quad  \text{in }\Omega_{\varepsilon}
\setminus\cup_{i=1}^{n+\tilde{n}+m+\tilde{m}}B_{i,R_1},\\
\frac{\partial}{\partial\nu}\psi\geq\sum_{i\in J_2\cup J_4}
\frac{\varepsilon_p}{v_i\rho_i}\frac{1}{|z_i|^{3+2\alpha}}+\varepsilon_p
\quad \text{on } \partial\Omega_{\varepsilon}\setminus\cup_{i\in J_2\cup J_4}B_{i,R_1},
\end{gathered}
\end{equation}
where   $-1<\alpha<\alpha_0$ and
$B_{i,R_1}=\{y\in\overline{\Omega}_{\varepsilon}:|z_i|<R_1\}$.
\end{lemma}


\begin{proof}
Following the proof of \cite[Lemma 3.4]{CY1}, we take
$$
g_{1i}(y)=\frac{(br_i)^{2(1+\alpha)}-1}{(br_i)^{2(1+\alpha)}+1},
\quad \text{for}\,\,i\in\cup_{l=1}^{4}J_l,\;
R_b\leq r_i\leq\delta(v_i\rho_i)^{-1},
$$
where  $b>0$, $r_i=|z_i|$  and
$R_b=\frac{1}{b}3^{\frac{1}{2(1+\alpha)}}$. Then  for $R_b\leq
r_i\leq\delta(v_i\rho_i)^{-1}$,
$$
-\Delta g_{1i}(y)+\varepsilon_p^2g_{1i}(y)
>\big(\frac{\varepsilon_p}{v_i\rho_i}\big)^2
b^{-2(1+\alpha)}\frac{4(1+\alpha)^2}{r_i^{2\alpha+4}},
$$
and by \eqref{2.19},
$$
W_q(y)\leq
C_1\big(\frac{\varepsilon_p}{v_i\rho_i}\big)^2\frac1{r_i^{2\alpha_{i}+4}}.
$$
So, if $b>0$ is sufficiently small so that
$4(1+\alpha)^2b^{-2(1+\alpha)}>C_1+1$, we have
\begin{equation}\label{3.8d}
L(g_{1i})(y)>\big(\frac{\varepsilon_p}{v_i\rho_i}\big)^2\frac{1}{r_i^{2\alpha+4}},
\end{equation}
and for $i\in J_2\cup J_4$,
\begin{equation}\label{3.8e}
|\frac{\partial }{\partial
\nu}g_{1i}(y)|\leq \frac{\varepsilon_p}{v_i\rho_{i}}\frac{C_{2}\delta}
{r_i^{3+2\alpha}}.
\end{equation}
We also take
$$
g_{2i}(y)=1-\frac{1}{r_i^{3+2\alpha}}\operatorname{Im}(z_i)\quad \text{for }i\in J_2\cup J_4,\;
R_b\leq r_i\leq\delta(v_i\rho_i)^{-1}.
$$
Then
\begin{gather}\label{3.8f}
L(g_{2i})(y)\geq (\frac{\varepsilon_p}{v_i\rho_i})^2
\big\{(1+2\alpha)(3+2\alpha)\frac{1}{r_i^{5+2\alpha}}
\operatorname{Im}(z_i)-C_1\frac{1}{r_i^{4+2\alpha_{i}}}\big\}, \\
\label{3.8g}
\frac{\partial}{\partial \nu}g_{2i}(y)
\geq\frac{\varepsilon_p}{v_i\rho_i}\frac{C_{3}}{r_i^{3+2\alpha}}.
\end{gather}
Consider now
$$
g_{3i}(y)=k_{1}g_{1i}(y)+g_{2i}(y)\quad \text{for }
i\in J_2\cup J_4,\,\,R_b\leq r_i\leq\delta(v_i\rho_i)^{-1},
$$
where $k_1$ is chosen larger and $\delta$ is chosen smaller if
necessary. It is easy to check that $|g_{3i}(y)|\leq C_{4}$ and
\[
|\nabla g_{3i}(y)|=O(\frac{\varepsilon_p}{v_i\rho_i}\frac{1}{r_i^{3+2\alpha}}).
\]
By \eqref{3.8d}-\eqref{3.8g}, we  find
\begin{gather}\label{3.8h}
L(g_{3i})(y)>(\frac{\varepsilon_p}{v_i\rho_i})^2\frac{1}{r_i^{4+2\alpha}}, \\
\label{3.8i}
\frac{\partial}{\partial \nu}g_{3i}(y)
>\frac{\varepsilon_p}{v_i\rho_i}\frac{C_{5}}{r_i^{3+2\alpha}}.
\end{gather}
Let $\eta_i(y)=\eta(v_i\rho_ir_i)$, where $\eta=\eta(t)$ is a smooth
cut-off function in $\mathbb{R}^2$ such that $\eta=1$ if
$t\leq\frac{1}{2}\delta$, $\eta=0$ if $t\geq\delta$.  Obviously, for
$\delta(2v_i\rho_i)^{-1}\leq r_i\leq\delta(v_i\rho_i)^{-1}$,
$|\nabla\eta_i(y)|\leq C_6\varepsilon_p$ and $|\Delta\eta_i(y)|\leq
C_6\varepsilon^2_p$. Besides, let
$g_{0}(y)=\tilde{g}(\varepsilon_p y)$, where $\tilde{g}$ is a
bounded positive  solution of
\begin{gather*}
-\Delta\tilde{g}+\tilde{g}=1\quad \text{in } \Omega,\\
\frac{\partial\tilde{g}}{\partial\nu}=1 \quad
\text{on }\partial\Omega,
\end{gather*}
so that $-\Delta g_0+\varepsilon_p^2g_0=\varepsilon_p^2$
in $\Omega_{\varepsilon}$,
$\frac{\partial}{\partial\nu}g_{0}=\varepsilon_p$  on
$\partial\Omega_{\varepsilon}$.
Moreover, $g_{0}(y)$ is uniformly bounded on
$\overline{\Omega}_{\varepsilon}$, i.e. $|g_{0}(y)|\leq C_7$.
Thus, for numbers $k_2,k_3$ and $R_1$ such that
$k_2>\max\{2,C_{5}^{-1}\}$,
$k_3>2+k_2C_6+k_2C_4C_6$
and
$R_{1}=\max\{R_b,(k_{3}C_{1}C_{7})^{\frac{1}{2(\alpha_{i}-\alpha)}}|\,i\in
\cup_{l=1}^{4}J_l\}$. The function
$$
\psi(y)=\sum_{i\in J_1\cup J_3}k_2\eta_{i}(y)g_{1i}(y)
+\sum_{i\in J_2\cup J_4}k_{2}\eta_{i}(y)g_{3i}(y)+k_{3}g_{0}(y)
$$
meets the requirements. The rest of the proof is similar to that of
\cite[Lemma 3.4]{CY1}, so we omit it.
\end{proof}


\begin{lemma} \label{lem3.3}
There exist  $C>0$  and $p_0>1$
such that for all $p>p_0$,  points $q\in\Lambda^{\tilde{m}}_{m}(\delta)$,
$h\in\mathcal {C}_{*}$,  and  $\phi$ the solution to
\begin{equation}\label{3.3r}
\begin{gathered}
L(\phi)=-\Delta \phi+\varepsilon_p^2\phi-W_q\phi=h\quad
\text{in }\Omega_{\varepsilon},\\
\frac{\partial\phi}{\partial\nu}=0\quad \text{on }
\partial\Omega_{\varepsilon},
\end{gathered}
\end{equation}
under the orthogonality conditions
\begin{equation}\label{3.7}
\begin{gathered}
\int_{\Omega_{\varepsilon}}\chi_i\,Z_{i0}\phi=0 \quad
\forall i\in J_1\cup J_2,\\
\int_{\Omega_{\varepsilon}}\chi_i Z_{ij}\phi=0
\quad \forall i\in J_3,\;j=0,1,2;\; i\in J_4,\; j=0,1,
\end{gathered}
\end{equation}
one has
\begin{equation}\label{3.8}
\|\phi\|_{\infty}\leq C\|h\|_{*}.
\end{equation}
\end{lemma}

\begin{proof}
First  we consider the ``inner norm''
$$
\|\phi\|_{R}=\sup_{y\in\overline{\Omega}_{\varepsilon}
\cap(\cup_{i=1}^{n+\tilde{n}+m+\tilde{m}}B_{i,R})}|\phi(y)|,
$$
we claim that there is a constant $C>0$ such that
\begin{equation}\label{3.9}
\|\phi\|_{\infty}\leq C(\|\phi\|_{R_1}+\|h\|_{*}),
\end{equation}
with $R_{1}$ given by Lemma \ref{lem3.2}.
Set
$$
\tilde{\phi}=C_1\psi(y)(\|\phi\|_{R_1}+\|h\|_{*})
\quad\forall y\in\overline{\Omega}_{\varepsilon}\setminus
\cup_{i=1}^{n+\tilde{n}+m+\tilde{m}}B_{i,R_1},
$$
where $\psi$ is the positive, uniformly bounded barrier constructed
by Lemma \ref{lem3.2} and $C_1>0$ is chosen larger if necessary.
Then for
$y\in\Omega_{\varepsilon}\setminus\cup_{i=1}^{n+\tilde{n}+m+\tilde{m}}B_{i,R_1}$,
\begin{align*}
L(\tilde{\phi}\pm\phi)(y)
&\geq C_{1}\,\|h\|_{*}\Big\{\sum_{i\in\cup_{l=1}^{4}
J_l}(\frac{\varepsilon_p}{v_i\rho_i})^2|\frac{\varepsilon_p
y-q_i}{v_i\rho_i}|^{-(4+2\alpha)}+\varepsilon_p^2\Big\}\pm
h(y)\\
&\geq|h(y)|\pm h(y)\geq0,
\end{align*}
for $y\in\partial\Omega_{\varepsilon}\setminus\cup_{i=1}^{n+\tilde{n}+m+\tilde{m}}B_{i,R_1}$,
$$
\frac{\partial}{\partial\nu}(\tilde{\phi}\pm\phi)(y)\geq 0,
$$
and for
$y\in\overline{\Omega}_{\varepsilon}\cap(\cup_{i=1}^{n+\tilde{n}
+m+\tilde{m}}\partial B_{i,R_1})$,
$$
(\tilde{\phi}\pm\phi)(y)>\|\phi\|_{R_1}\pm\phi(y)\geq
|\phi(y)|\pm\phi(y)\geq 0.
$$
From  the maximum principle (see
\cite{PW}), it follows that
$-\tilde{\phi}(y)\leq\phi(y)\leq\tilde{\phi}(y)$ on
$\overline{\Omega}_{\varepsilon}\setminus
\cup_{i=1}^{n+\tilde{n}+m+\tilde{m}}B_{i,R_1}$,
which implies that \eqref{3.9} holds.

Let us  prove the  a priori estimate \eqref{3.8}  by contradiction. We
assume the existence of   sequences $p_j\to+\infty$,
functions $h_j$ with $\|h_j\|_{*}\to 0$, points
$q^j=(q^j_{n+\tilde{n}+1},\ldots,q^j_{n+\tilde{n}+m+\tilde{m}})
\in\Lambda^{\tilde{m}}_{m}(\delta)$,
solutions $\phi_j$
with $\|\phi_j\|_\infty=1$ such that \eqref{3.3r}-\eqref{3.7} holds.
From  estimate  \eqref{3.9},
$\sup_{\overline{\Omega}_{\varepsilon}\cap B_{i,R_1}}|\phi_j|\geq\kappa>0$
for some $i$ and $\kappa$.
To simplify the notation, let us set $p=p_j$, $\varepsilon_p=\varepsilon_{p_j}$
and $q_i=q_i^j$. Set
$\hat{\phi}_j(z)=\phi_j(\frac{v_i\rho_i}{\varepsilon_p}z+\frac{q_i}{\varepsilon_p})$
and
$\hat{h}_j(z)=h_j(\frac{v_i\rho_i}{\varepsilon_p}z+\frac{q_i}{\varepsilon_p})$.
While $q_i\in\Omega$, $i\in J_1\cup J_3$,
by \eqref{2.18c},
$\hat{\phi}_j$ satisfies
$$
-\Delta\hat{\phi}_j+(v_i\rho_i)^2\hat{\phi}_j
-\frac{8(1+\alpha_i)^2|z|^{2\alpha_i}}{[1+|z|^{2(1+\alpha_i)}]^2}
[1+O(\frac1p)\,]\hat{\phi}_j=(\frac{v_i\rho_i}{\varepsilon_p})^2\,\widehat{h}_j,
$$
for $z\in B_{R_1}(0)$. Obviously, for any $\beta\in [1,-\frac1{\alpha}]$,
$(\frac{v_i\rho_i}{\varepsilon_p})^2\hat{h}_j\to 0$ in
$L^\beta(B_{R_1}(0))$. Since
$\frac{8(1+\alpha_{i})^2|z|^{2\alpha_{i}}}{[1+|z|^{2(1+\alpha_i)}]^2}$
is bounded in $L^\beta(B_{R_1}(0))$ and
$\|\hat{\phi}_j\|_{\infty}=1$, elliptic regularity theory
readily implies that $\hat{\phi}_j$ converges uniformly over
compact subsets near the origin to a bounded nontrivial solution
$\hat{\phi}$ of  $L_i(\hat{\phi})=0$ in $\mathbb{R}^2$.
Then $\hat{\phi}$ is
proportional to $z_{i0}$ for  $i\in J_1$,  or a linear combination
of $z_{i0}$, $z_{i1}$ and $z_{i2}$ for $i\in J_3$. However,
our assumed orthogonality conditions \eqref{3.7}  on $i$ and
$\phi_j$, pass to limit and yield $\int\chi
z_{i0}\hat{\phi}dz=0$ for $i\in J_1$, or
$\int\chi z_{il}\hat{\phi}dz=0$ for
$i\in J_3,\,l=0,1,2$, which implies  $\hat{\phi}\equiv0$.
This is absurd because $\hat{\phi}$ is nontrivial.

While $q_i\in\partial\Omega,\,i\in J_2\cup J_4$, $\hat{\phi}_j$
satisfies
\begin{gather*}
-\Delta\hat{\phi}_j+(v_i\rho_i)^2\hat{\phi}_j
-\frac{8(1+\alpha_i)^2|z|^{2\alpha_i}}{[1+|z|^{2(1+\alpha_i)}]^2}
[1+O(\frac1p)]\hat{\phi}_j=\big(\frac{v_i\rho_i}{\varepsilon_p}\big)^2\\
\hat{h}_j\quad \text{in } B_{R_1}(0)\cap\Omega_{v_i\rho_i},\\
\frac{\partial}{\partial\nu}\hat{\phi}_j=0\quad
\text{on } B_{R_1}(0)\cap\partial\Omega_{v_i\rho_i},
\end{gather*}
where $\Omega_{v_i\rho_i}=\frac{1}{v_i\rho_i}(\Omega-\{q_i\})$. Obviously,
for any $\beta\in[1,-\frac1{\alpha}]$,
$(\frac{v_i\rho_i}{\varepsilon_p})^2\hat{h}_j\to 0$ in
$L^\beta(B_{R_1}(0)\cap\Omega_{v_i\rho_i})$. Since
$\frac{8(1+\alpha_{i})^2|z|^{2\alpha_i}}{[1+|z|^{2(1+\alpha_i)}]^2}$
is bounded in $L^\beta(B_{R_1}(0)\cap\Omega_{v_i\rho_i})$ and
$\|\hat{\phi}_j\|_{\infty}=1$, elliptic regularity theory
readily implies that  $\hat{\phi}_j$ converges uniformly on
$B_{R_1}(0)\cap\overline{\Omega}_{v_i\rho_i}$ to a bounded nontrivial
solution $\hat{\phi}$ of  $L_i(\hat{\phi})=0$ in $\mathbb{R}^2_+$ and
$\frac{\partial
}{\partial z_2}\hat{\phi}(z_1,0)=0$ on $\partial\mathbb{R}^2_+$.
Then  $\hat{\phi}$ is proportional to $z_{i0}$ for $i\in J_2$, or
a linear combination of  $z_{i0}$ and $z_{i1}$ for $i\in J_4$.
However, our assumed orthogonality conditions \eqref{3.7} on
$i$ and $\phi_j$, pass to limit and easily yield $\int\chi
z_{i0}\hat{\phi}=0$ for  $i\in J_2$, or $\int\chi
z_{il}\hat{\phi}dz=0$ for $i\in
J_4,\,l=0,1$, which implies $\hat{\phi}\equiv0$.
This is also absurd because $\hat{\phi}$ is nontrivial, which
completes the proof.
\end{proof}

\begin{lemma} \label{lem3.4}
 There exist   $C>0$  and $p_0>1$
 such that for any $p>p_0$,  points $q\in\Lambda^{\tilde{m}}_{m}(\delta)$,
$h\in\mathcal {C}_{*}$,  and  solution $\phi$ of \eqref{3.3r}
with
\begin{equation}\label{3.10}
\int_{\Omega_{\varepsilon}}\chi_iZ_{ij}\phi=0
\quad \forall i\in J_3,\; j=1,2;\; i\in J_4,\;j=1,
\end{equation}
one has
\begin{equation}\label{3.11}
\|\phi\|_{\infty}\leq Cp\|h\|_{*}.
\end{equation}
\end{lemma}

\begin{proof}
Let $R>R_0+1$ be large and fixed. For
$i\in \cup_{l=1}^{4}J_l$, denote
\begin{gather*}
a_{i0}=\frac1{\mu_i[H(q_i,q_i)-\frac{1}{d_i}4(1+\alpha_i)\log(v_i\rho_i R)]}, \\
\widehat{Z}_{i0}(y)=Z_{i0}(y)-\frac1{\mu_i}
+a_{i0}G(q_i,\varepsilon_p y).
\end{gather*}
Let   $\eta_1$ and $\eta_2$ be  radial smooth cut-off functions in
 $\mathbb{R}^2$ such that
\begin{gather*}
0\leq\eta_1\leq1;\quad |\nabla\eta_1|\leq C\,\,\text{in}\,\mathbb{R}^2;
\quad \eta_1\equiv1\text{ in }B_R(0);\quad
\eta_1\equiv0 \text{ in } \mathbb{R}^2\setminus B_{R+1}(0);\\
0\leq\eta_2\leq1;\quad |\nabla\eta_2|\leq C\text{ in }\mathbb{R}^2;\quad
\eta_2\equiv1\text{ in } B_{\frac{\kappa}{4}\delta}(0);\quad
\eta_2\equiv0\text{ in }\mathbb{R}^2\setminus B_{\frac{\kappa}3\delta}(0),
\end{gather*}
where $0<\kappa\leq1$ will be chosen later on.
Set
\begin{gather*}
\eta_{1i}(y)=\eta_1(|\tilde{z}_i(y)|),\quad
\eta_{2i}(y)=\eta_2(v_i\rho_i|\tilde{z}_i(y)|), \\
\widetilde{Z}_{i0}(y)=\eta_{1i}Z_{i0}+(1-\eta_{1i})\eta_{2i}\widehat{Z}_{i0}.
\end{gather*}
Now define
\begin{equation}\label{3.11t}
\widetilde{\phi}=\phi+\sum_{i=1}^{n+\tilde{n}+m+\tilde{m}}e_i\widetilde{Z}_{i0},
\end{equation}
where  $e_i$ is chosen such
that for any $i\in\cup_{l=1}^4J_l$,
$$
e_i\int_{\Omega_{\varepsilon}}\chi_i|Z_{i0}|^2
+\int_{\Omega_{\varepsilon}}\chi_iZ_{i0}\phi=0,
$$
Note that $\frac{\partial}{\partial\nu}\widetilde{Z}_{i0}=0$
for any $i\in J_2\cup J_4$,
which arises from $\frac{\partial}{\partial z_2}z_{i0}(z_1,0)=0$ and
$F_i$ preserves the Neumann boundary condition.
Thus
\begin{equation}\label{3.12}
\begin{gathered}
L(\widetilde{\phi})=h+\sum_{i=1}^{n+\tilde{n}+m
+\tilde{m}}e_i\,L(\widetilde{Z}_{i0})
\quad\text{in }\Omega_{\varepsilon},\\
\frac{\partial\widetilde{\phi}}{\partial\nu}=0 \quad \text{on }
\partial\Omega_{\varepsilon},
\end{gathered}
\end{equation}
and $\widetilde{\phi}$ satisfies the orthogonality conditions
\eqref{3.7}. By \eqref{3.8}, it implies that
\begin{equation}\label{3.13}
\|\widetilde{\phi}\|_\infty\leq\,
C\big\{\|h\|_*+\sum_{i=1}^{n+\tilde{n}+m
+\tilde{m}}|e_i|\cdot\|L(\widetilde{Z}_{i0})\|_{*}\big\}.
\end{equation}
Multiplying \eqref{3.12} by
$\widetilde{Z}_{i0}$, $i\in\cup_{l=1}^4J_l$, and integrating by parts,
it follows that
\begin{equation}\label{3.134}
\langle L(\widetilde{Z}_{i0}),\widetilde{\phi}\rangle
=\langle\widetilde{Z}_{i0},h\rangle+e_i\langle
L(\widetilde{Z}_{i0}),\widetilde{Z}_{i0}\rangle,
\end{equation}
where $\langle f,g\rangle=\int_{\Omega_\varepsilon}fg$.
Then for $i\in\cup_{l=1}^{4}J_l$, by \eqref{3.13}-\eqref{3.134},
$$
|e_i\langle L(\widetilde{Z}_{i0}),\widetilde{Z}_{i0}\rangle|
\leq C\|h\|_{*}(1+\|L(\widetilde{Z}_{i0})\|_{*})
+C\|L(\widetilde{Z}_{i0})\|_{*}\sum_{i=1}^{n+\tilde{n}+m
+\tilde{m}}|e_j|\cdot\|L(\widetilde{Z}_{j0})\|_{*}.
$$
Let us claim that for any $i\in\cup_{l=1}^{4}J_l$,
\begin{gather}
\|L(\widetilde{Z}_{i0})\|_{*}=O(\frac1p), \label{3.15}\\
\langle L(\widetilde{Z}_{i0}),\widetilde{Z}_{i0}\rangle
=-\frac{C}{p}\big\{1+O(\frac{\log R}{R^{2(1+\alpha_i)}})\big\}.\label{3.16}
\end{gather}
Once these estimates are proven, it easily follows that
\begin{equation}\label{3.17}
|e_i|\leq Cp\,\|h\|_{*}.
\end{equation}
This, together with \eqref{3.11t}, \eqref{3.13} and
\eqref{3.15},  implies   estimate \eqref{3.11} for $\phi$.

\noindent \textbf{Proof of \eqref{3.15}.}
For sake of simplicity, we only
prove  estimate $\eqref{3.15}$ for any $i\in J_2\cup J_4$. Since
 $\nabla F_i(q_i)=Id$, it follows that
\begin{gather}
z_i=\frac{\varepsilon_p y-q_i}{v_i\rho_i}
=\frac{\varepsilon_p\tilde{F}_i^\varepsilon(\tilde{z}_i)-q_i}{v_i\rho_i}
=\tilde{z}_i\{1+O(v_i\rho_i\tilde{z}_i)\}, \label{3.53a}\\
\tilde{z}_i=F_i^\varepsilon(y)
=\frac{F_i(v_i\rho_i z_i+q_i)}{v_i\rho_i}=z_i\{1+O(v_i\rho_iz_i)\},
\label{3.53a1}\\
\Delta_y=(\frac{\varepsilon_p}{v_i\rho_i})^2\{\Delta_{\tilde{z}_i}
+O(\rho_i|\tilde{z}_i|) \nabla_{\tilde{z}_i}^2+O(\rho_i)\nabla_{\tilde{z}_i}\}.
\label{3.53c}
\end{gather}
So, $\kappa\leq1$ can be  chosen such  that if
$|\tilde{z}_i|\leq\frac13\kappa\delta(v_i\rho_i)^{-1}$,
then $|z_i|\leq\delta(v_i\rho_i)^{-1}$.
Note that
\begin{equation}\label{3.14}
\begin{aligned}
L(\widetilde{Z}_{i0})
&=\eta_{1i}LZ_{i0}+(1-\eta_{1i})\eta_{2i}L\widehat{Z}_{i0}
+2\nabla\eta_{1i}\nabla Z_{i0}+Z_{i0}\Delta\eta_{1i}\\
& \quad +2\nabla\widehat{Z}_{i0}\nabla[(1-\eta_{1i})\eta_{2i}]
+\widehat{Z}_{i0}\Delta[(1-\eta_{1i})\eta_{2i}].
\end{aligned}
\end{equation}
For $r_i:=|\tilde{z}_i|\leq R+1$,  by \eqref{2.18c}, \eqref{3.2b}
and \eqref{3.53a},
$$
L(Z_{i0})=(W_q-W_{i0})Z_{i0}+O(\frac{\varepsilon_p^2}{v_i\rho_i}\frac{
|z_i|^{2\alpha_i}}{(1+|z_i|)^{3+4\alpha_i}})-\varepsilon_p^2Z_{i0},
$$
which implies
\begin{equation}\label{3.15b}
\|\eta_{1i}L(Z_{i0})\|_{*}=O(\frac1p).
\end{equation}
Note that for $ r_i\geq R$,  by \eqref{3.53a}-\eqref{3.53a1},
\begin{gather}
|Z_{i0}-\frac1{\mu_i}|\leq\,C(1+|\tilde{z}_i|)^{-2(1+\alpha_i)}
=O(|z_i|^{-2(1+\alpha_i)}), \label{3.15c}\\
|a_{i0}G(q_i,\varepsilon_p y)-\frac1{\mu_i}|
\leq \frac{C(1+\log\frac{|z_i|}R)}
{H(q_i,q_i)-\frac1{d_i}4(1+\alpha_i)\log(v_i\rho_i R)}=O
(\frac{1+\log\frac{|z_i|}R}p).\label{3.15d}
\end{gather}
For $R\leq r_i\leq\frac13\kappa\delta(v_i\rho_i)^{-1}$, by \eqref{3.2b},
$$
L(\widehat{Z}_{i0})=W_q[a_{i0}G(q_i,\varepsilon_p y)-\frac1{\mu_i}]
+[W_q-W_{i0}]Z_{i0}-\varepsilon_p^2(Z_{i0}-\frac1{\mu_i})
+O(\frac{\varepsilon^2_p}{v_i\rho_i|z_i|^{3+2\alpha_i}}),
$$
which, together with \eqref{2.19},  \eqref{3.15c} and \eqref{3.15d},
easily indicates that
\begin{equation}\label{3.15e}
\|(1-\eta_{1i})\eta_{2i}L(\widehat{Z}_{i0})\|_{*}=O(\frac1p).
\end{equation}
For $R\leq r_i\leq R+1$,
\begin{equation}\label{3.15j}
Z_{i0}-\widehat{Z}_{i0}
=\frac1{\mu_i}-a_{i0}G(q_i,\varepsilon_p y)=\frac{H(q_i,q_i)
-H(q_i,\varepsilon_p y)+
\frac{4(1+\alpha_i)}{d_i}\log\frac{|z_i|}R}{\mu_i[H(q_i,q_i)
-\frac{4(1+\alpha_i)}{d_i}\log(v_i\rho_i R)]},
\end{equation}
which, together with \eqref{3.53c}, implies that
\begin{gather}\label{3.15f}
(Z_{i0}-\widehat{Z}_{i0})\Delta\eta_{1i}=
O(\frac1p)(\frac{\varepsilon_p}{v_i\rho_i})^2\{\eta''_1(r_i)
+\frac1{r_i}\eta'_1(r_i)+O(\rho_i)\}, \\
\label{3.15g}
\nabla\eta_{1i}\nabla(Z_{i0}-\widehat{Z}_{i0})
=-(\frac{\varepsilon_p}{v_i\rho_i})^2
\frac{\eta_1'}{\mu_i\log(v_i\rho_iR)}\frac1{r_i}\,\{1+O(\frac1p)\}.
\end{gather}
Thus,
\begin{equation}\label{3.15a}
\|2\nabla\eta_{1i}\nabla(Z_{i0}-\widehat{Z}_{i0})+(Z_{i0}
-\widehat{Z}_{i0})\Delta\eta_{1i}\|_{*}=O(\frac1p).
\end{equation}
For $\frac14\kappa\delta(v_i\rho_i)^{-1}\leq r_i
\leq \frac13\kappa\delta(v_i\rho_i)^{-1}$,
it follows that $\widehat{Z}_{i0}=O(\frac1p)$
and $\nabla\widehat{Z}_{i0}=O(\frac{\varepsilon_p}p)$.
Then
\begin{equation}\label{3.15i}
\|\widehat{Z}_{i0}\Delta\eta_{2i}+2\nabla\widehat{ Z}_{i0}\nabla\eta_{2i}\|_{*}
=O(\frac1p).
\end{equation}
Joining  \eqref{3.14}, \eqref{3.15b}, \eqref{3.15e}, \eqref{3.15a} and
\eqref{3.15i}, we obtain that
\eqref{3.15} holds for $i\in J_2\cup J_4$.
\smallskip

\noindent\textbf{Proof of \eqref{3.16}.}
Note that for any $i\in\cup_{l=1}^{4}J_l$,
$\langle L(\widetilde{Z}_{i0}),\widetilde{Z}_{i0}\rangle=I+K$,
where
\begin{align*}
I&=\int_{\Omega_\varepsilon}\widetilde{Z}_{i0}
\{\eta_{1i}L Z_{i0}+(1-\eta_{1i})\eta_{2i}L\widehat{Z}_{i0}\}\\
&=\int_{\Omega_\varepsilon}\eta_{2i}^2\big\{Z_{i0}+(1-\eta_{1i})
[a_{i0}G(q_i,\varepsilon_p y)-\frac1{\mu_i}]\big\}
\Big\{(W_q-W_{i0})Z_{i0}+(\Delta Z_{i0}\\
&\quad +W_{i0}Z_{i0})
+(1-\eta_{1i})W_q[a_{i0}G(q_i,\varepsilon_p y)-\frac1{\mu_i}]
-\varepsilon_p^2(Z_{i0}-\frac1{\mu_i}+\frac{1}{\mu_i}\eta_{1i})\Big\},
\end{align*}
and
\[
K=\int_{\Omega_{\varepsilon}}\widetilde{Z}_{i0}\{Z_{i0}\Delta\eta_{1i}
+\widehat{Z}_{i0}\Delta[(1-\eta_{1i})\eta_{2i}]+2\nabla Z_{i0}\nabla\eta_{1i}
+2\nabla\widehat{Z}_{i0}\nabla[(1-\eta_{1i})\eta_{2i}]\}.
\]
For $R\leq r_i=|\tilde{z}_i|\leq\frac13\kappa\delta(v_i\rho_i)^{-1}$,
by \eqref{2.19}, \eqref{3.53a}, \eqref{3.53a1} and \eqref{3.15d},
\begin{align*}
&\int_{\Omega_{\varepsilon}}\eta_{2i}^2(1-\eta_{1i})\{Z_{i0}+(1-\eta_{1i})[a_{i0}G(q_i,\varepsilon_p y)-\frac1{\mu_i}]\}
W_q[a_{i0}G(q_i,\varepsilon_p y)-\frac1{\mu_i}]\\
&=O(\frac{\log R}{pR^{2(1+\alpha_i)}}).
\end{align*}
By \eqref{3.2b} and \eqref{3.15d},
$$
\int_{\Omega_{\varepsilon}}\eta_{2i}^2\{Z_{i0}+(1-\eta_{1i})
[a_{i0}G(q_i,\varepsilon_p y)-\frac1{\mu_i}]\}(\Delta Z_{i0}
+W_{i0}Z_{i0})=O(\rho_i+\varepsilon_p^2).
$$
By \eqref{3.15c}-\eqref{3.15d},
$$
\varepsilon_p^2\int_{\Omega_{\varepsilon}}\eta_{2i}^2\{Z_{i0}
+(1-\eta_{1i})
[a_{i0}G(q_i,\varepsilon_p y)-\frac1{\mu_i}]\}(Z_{i0}-\frac1{\mu_i})
=O(\rho_i^2+\varepsilon_p^2).
$$
Furthermore,
\begin{equation}\label{3.16d}
I=\int_{\Omega_{\varepsilon}}\eta_{2i}^2(W_q-W_{i0})Z^2_{i0}
dy +O(\frac{\log R}{pR^{2(1+\alpha_i)}})+O(\rho_i+\varepsilon_p^2).
\end{equation}
By \eqref{2.5c}, a straightforward but tedious computation shows that
\begin{gather}\label{3.16f}
\int_{\mathbb{R}^2}(\frac{\varepsilon_p}{v_i\rho_i})^2|z_i|^{2\alpha_i}e^{U^i(z_i)}
\frac{\omega^{0i}-U^i-\frac12(U^i)^2}pz^2_{i0}(z_i)dy
=-\frac{8\pi(\alpha_i+1)}{p\mu_i^2}, \\
\label{3.16g}
\int_{|z_i|\geq\delta(v_i\rho_i)^{-1/2}}(\frac{\varepsilon_p}{v_i\rho_i})^2
|z_i|^{2\alpha_i}e^{U^i(z_i)}
\frac{\omega^{0i}-U^i-\frac12(U^i)^2}pz^2_{i0}(z_i)dy
=O(\frac1p\varepsilon_p^{\frac12}).
\end{gather}
By \eqref{3.53a}-\eqref{3.53a1}, it easily follows that for
 $|z_i|\leq\delta(v_i\rho_i)^{-1/2}$,
\begin{equation}\label{3.16g1}
Z_{i0}(y)=z_{i0}(\tilde{z}_i)=z_{i0}(z_i)[1+O(\rho_i|z_i|)].
\end{equation}
This,  together with  \eqref{2.18c} and \eqref{3.16f}-\eqref{3.16g1},
easily indicates that
\begin{equation}\label{3.16h}
\int_{|z_i|\leq\delta(v_i\rho_i)^{-1/2}}\eta_{2i}^2(W_q-W_{i0})Z^2_{i0}=
\begin{cases}
-\frac{8\pi(\alpha_i+1)}{p\mu_i^2}
+O(\frac1{p^2}) & \forall \,i\in J_1\cup J_3,\\
-\frac{4\pi(\alpha_i+1)}{p\mu_i^2}
+O(\frac1{p^2}) & \forall \,i\in J_2\cup J_4.
\end{cases}
\end{equation}
Also by  \eqref{2.19},
\begin{equation}\label{3.16e}
\int_{|z_i|\geq\delta(v_i\rho_i)^{-1/2}}\eta_{2i}^2(W_q-W_{i0})Z^2_{i0}
=\int_{|z_i|\geq\delta(v_i\rho_i)^{-1/2}}O(\frac1{|z_i|^{4+2\alpha_i}})
=O(\varepsilon_p).
\end{equation}
So, by  \eqref{3.16d}, \eqref{3.16h} and \eqref{3.16e}, it follows  that
\begin{equation}\label{3.16i}
I=\begin{cases}
-\frac{8\pi(\alpha_i+1)}{p\mu_i^2}
+O(\frac{\log R}{pR^{2(1+\alpha_i)}}) &\forall \,i\in J_1\cup J_3,\\
-\frac{4\pi(\alpha_i+1)}{p\mu_i^2}
+O(\frac{\log R}{pR^{2(1+\alpha_i)}}) &\forall \,i\in J_2\cup J_4.
\end{cases}
\end{equation}

Let us give the estimate of $K$.
Integrating by parts  the first two terms of $K$,
\begin{align*}
K&=\int_{\Omega_{\varepsilon}}
\widetilde{Z}_{i0}\nabla Z_{i0}\nabla\eta_{1i}
-Z_{i0}\nabla\widetilde{Z}_{i0}\nabla\eta_{1i}
+\widetilde{Z}_{i0}\nabla\widehat{Z}_{i0}\nabla[(1-\eta_{1i})\eta_{2i}]\\
&\quad -\widehat{Z}_{i0}\nabla\widetilde{Z}_{i0}\nabla[(1-\eta_{1i})\eta_{2i}]\\
&=K_1+K_2,
\end{align*}
where
\begin{align*}
K_1&=\int_{R\leq|\tilde{z}_i|\leq R+1}
\widetilde{Z}_{i0}\nabla Z_{i0}\nabla\eta_{1i}-Z_{i0}\nabla\widetilde{Z}_{i0}
 \nabla\eta_{1i}
-\widetilde{Z}_{i0}\nabla\widehat{Z}_{i0}\nabla\eta_{1i}
+\widehat{Z}_{i0}\nabla\widetilde{Z}_{i0}\nabla\eta_{1i}\\
&=\int_{R\leq|\tilde{z}_i|\leq R+1}\,\,Z_{i0}\nabla(Z_{i0}
 -\widehat{Z}_{i0})\nabla\eta_{1i}
+(\widehat{Z}_{i0}-Z_{i0})\nabla(Z_{i0}-\widehat{Z}_{i0})\nabla\eta_{1i}\\
&\quad -(Z_{i0}-\widehat{Z}_{i0})\nabla\widehat{Z}_{i0}\nabla\eta_{1i}-(Z_{i0}
-\widehat{Z}_{i0})^2|\nabla\eta_{1i}|^2,
\end{align*}
and
\[
K_2= \int_{\frac{\kappa\delta}{4v_i\rho_i}\leq|\tilde{z}_i|
\leq \frac{\kappa\delta}{3v_i\rho_i}}
(\widetilde{Z}_{i0}\nabla\widehat{Z}_{i0}
-\widehat{Z}_{i0}\nabla\widetilde{Z}_{i0})\nabla\eta_{2i}
=-\int_{\Omega_{\varepsilon}}
|\widehat{Z}_{i0}|^2|\nabla\eta_{2i}|^2=O(\frac1{p^2}).
\]
Note that for $R\leq|\tilde{z}_i|\leq R+1$,  by \eqref{3.53a}-\eqref{3.53a1},
$|\nabla\widehat{Z}_{i0}|=\frac{\varepsilon_p}{v_i\rho_i}
\{O(\frac1{R^{2(1+\alpha_i)+1}})+O(\frac1{pR})\}$.
By \eqref{3.15j} and \eqref{3.15g}, it follows that
\begin{gather*}
\int_{R\leq|\tilde{z}_i|\leq R+1}(Z_{i0}
-\widehat{Z}_{i0})^2|\nabla\eta_{1i}|^2dy=O(\frac1{p^2}),
\\
\int_{R\leq|\tilde{z}_i|\leq R+1}(\widehat{Z}_{i0}-Z_{i0})
\nabla(Z_{i0}-\widehat{Z}_{i0})\nabla\eta_{1i}dy=O(\frac1{p^2}),
\\
\int_{R\leq|\tilde{z}_i|\leq R+1}(Z_{i0}-\widehat{Z}_{i0})
\nabla\widehat{Z}_{i0}\nabla\eta_{1i}dy
=O(\frac1p\cdot\frac1{R^{2(1+\alpha_i)+1}}).
\end{gather*}
Thus
$$
K=K_1+K_2=\int_{R\leq|\tilde{z}_i|\leq R+1}Z_{i0}
\nabla(Z_{i0}-\widehat{Z}_{i0})\nabla\eta_{1i}dy
+O(\frac1p\cdot\frac1{R^{2(1+\alpha_i)+1}}),
$$
which, together with \eqref{3.53a}, \eqref{3.53a1} and \eqref{3.15g},
implies   that
\begin{equation}\label{3.16j1}
K=\begin{cases}
-\frac{2\pi}{\mu_i^2|\log(v_i\rho_iR)|}\{1+O(\frac{1}{R^{2(1+\alpha_i)}})\}
&\forall i\in J_1\cup J_3,\\
-\frac{\pi}{\mu_i^2|\log(v_i\rho_iR)|}\{1+O(\frac{1}{R^{2(1+\alpha_i)}})\}
& \forall i\in J_2\cup J_4.
\end{cases}
\end{equation}
As a consequence,  estimate \eqref{3.16} can be  derived from
 \eqref{3.16i}-\eqref{3.16j1}.
\end{proof}


\begin{proof}[Proof of Proposition \ref{prop3.1}]
Let us prove  \eqref{3.5} by contradiction.
Assume that as $p_l\to + \infty$,
\begin{equation}\label{3.5j}
\|\phi_l\|_{\infty}=1,\quad p_l\|h_l\|_*\to0,\quad
p_l\Big(\sum_{i\in J_3\cup J_4}|c^l_{i1}|
+\sum_{i\in J_3}|c^l_{i2}|\Big)\geq\kappa>0.
\end{equation}
For convenience, we omit the dependence on $l$.
By \eqref{3.11},
\begin{equation}\label{3.5f}
\|\phi\|_{\infty}\leq Cp\big\{\|h\|_{*}+
\sum_{i\in J_3\cup J_4}|c_{i1}|
+\sum_{i\in J_3}|c_{i2}|\big\}.
\end{equation}
Testing equation  \eqref{3.3}  against $\eta_{2i}Z_{ij}$ with
$i\in J_3$, $j=1,2$, or  $i\in J_4$, $j=1$, and integrating by parts,
it implies that
\begin{equation}\label{3.5b}
|c_{ij}|\leq C\big\{|\langle
\phi,\,L(\eta_{2i}Z_{ij})\rangle|+|\langle h,\,\eta_{2i}Z_{ij}\rangle|\big\}.
\end{equation}
By \eqref{3.53c}, it follows that for
$|\tilde{z}_i|\leq\frac13\kappa\delta(v_i\rho_i)^{-1}$,
\begin{align*}
L(\eta_{2i}Z_{ij})
&=\eta_2(v_i\rho_i\tilde{z}_i)z_{ij}(\tilde{z}_i)
\big\{W_q-(\frac{\varepsilon_p}{v_i\rho_i})^2\frac{8(1+\alpha_i)^2
|\tilde{z}_i|^{2\alpha_i}}{[1+|\tilde{z}_i|^{2(1+\alpha_i)}]^2}\big\}\\
&\quad +\big(\frac{\varepsilon_p}{v_i\rho_i}\big)^2
\big\{O(\rho_i|\tilde{z}_i|)\nabla_{\tilde{z}_i}^2z_{ij}
+O(\rho_i)\nabla_{\tilde{z}_i}z_{ij}+O(\rho^2_i)z_{ij}\big\}(\tilde{z}_i).
\end{align*}
Note that
$|z_{ij}|=O((1+|\tilde{z}|)^{-1-\alpha_i})$,
$|\nabla_{\tilde{z}_i} z_{ij}|=O((1+|\tilde{z}|)^{-2-\alpha_i})$ and
$|\nabla^2_{\tilde{z}_i}z_{ij}|=O((1+|\tilde{z}|)^{-3-\alpha_i})$.
This combined \eqref{2.19}-\eqref{2.18c} and  \eqref{3.53a}-\eqref{3.53a1}
implies that  for
$|\tilde{z}_i|\leq\frac12\delta(v_i\rho_i)^{-1/2}$,
\begin{align*}
&L(\eta_{2i}Z_{ij})\\
&=\big(\frac{\varepsilon_p}{v_i\rho_i}\big)^2|
 \tilde{z}_i|^{2\alpha_i}z_{ij}(\tilde{z}_i)e^{U^i(\tilde{z}_i)}
\big\{\frac{[\omega^{0i}-U^i-\frac12(U^i)^2](|\tilde{z}_i|)}p
+O(\frac{\log^4(2+|\tilde{z}_i|)}{p^2})\big\}\\
&\quad +\,(\frac{\varepsilon_p}{v_i\rho_i})^2
\big\{O(\frac{|\tilde{z}_i|^{2\alpha_i}}{(1+|\tilde{z}_i|)^{5(1+\alpha_i)}})
+O(\frac{\rho_i}{(1+|\tilde{z}_i|)^{2+\alpha_i}})
+O(\frac{\rho^2_i}{(1+|\tilde{z}_i|)^{1+\alpha_i}})\big\},
\end{align*}
and for
$\frac12\delta(v_i\rho_i)^{-1/2}\leq|\tilde{z}_i|
\leq\frac13\kappa\delta(v_i\rho_i)^{-1}$,
$$
L(\eta_{2i}Z_{ij})
=(\frac{\varepsilon_p}{v_i\rho_i})^2O(\frac{1}{(1+|\tilde{z}_i|)^{5+3\alpha_i}}
+\frac{\rho_i}{(1+|\tilde{z}_i|)^{2+\alpha_i}}
+\frac{\rho^2_i}{(1+|\tilde{z}_i|)^{1+\alpha_i}}).
$$
This implies that for any
$i\in J_3$, $j=1,2$, or  $i\in J_4$, $j=1$,
\begin{equation}\label{3.5d}
\langle \phi, L(\eta_{2i}Z_{ij})\rangle
=\frac1p\,E_{ij}(\hat{\phi}_i)+O(\frac{\|\phi\|_{\infty}}{p^2}),
\end{equation}
where
\[
\hat{\phi}_i(\tilde{z}_i)=\begin{cases}
\phi(\frac{v_i\rho_iz_i+q_i}{\varepsilon_p}) & \forall  i\in J_3,\\
\phi(\tilde{F}_i^\varepsilon(\tilde{z}_i))
&  \forall i\in J_4,
\end{cases}
\]
and for $i\in J_3$,
\begin{gather*}
E_{i1}(\hat{\phi}_i)=\int_{B(0,\frac12\delta(v_i\rho_i)^{-1/2})}
\frac{32\operatorname{Re}(z_i)[\omega^{0i}-U^i-\frac{1}2(U^i)^2]}
{[1+|z_i|^2]^3}\hat{\phi}_i
dz_i,\\
E_{i2}(\hat{\phi}_i)=\int_{B(0,\frac12\delta(v_i\rho_i)^{-1/2})}
\frac{32\operatorname{Im}(z_i)[\omega^{0i}-U^i-\frac{1}2(U^i)^2]}
{[1+|z_i|^2]^3}\hat{\phi}_i
dz_i,
\end{gather*}
and for $i\in J_4$, by  \eqref{3.53a}-\eqref{3.53a1},
\begin{align*}
E_{i1}(\hat{\phi}_i)
&=\int_{\mathbb{R}_+^2\cap B(0,\frac12\delta(v_i\rho_i)^{-1/2})}
\frac{32\operatorname{Re}(\tilde{z}_i)[\omega^{0i}-U^i-\frac{1}2(U^i)^2]}
{[1+|\tilde{z}_i|^2]^3}\hat{\phi}_i\det[D\tilde{F}_i(\tilde{z}_i)]d\tilde{z}_i\\
&=\int_{\mathbb{R}_+^2\cap B(0,\frac12\delta(v_i\rho_i)^{-1/2})}
\frac{32\operatorname{Re}(\tilde{z}_i)[\omega^{0i}-U^i-\frac{1}2(U^i)^2]}
{[1+|\tilde{z}_i|^2]^3}\hat{\phi}_id\tilde{z}_i+O(\varepsilon_p\|\phi\|_{\infty}).
\end{align*}
Also
\begin{equation}\label{3.5c}
\langle h,\,\eta_{2i}Z_{ij}\rangle=O(\|h\|_*)=o(\frac1p).
\end{equation}
Substituting   \eqref{3.5d}-\eqref{3.5c} in \eqref{3.5b}, it
follows that
\begin{equation}\label{3.5e}
|c_{ij}|=O(\|h\|_*)+O(\frac{|\phi\|_\infty}p).
\end{equation}
Furthermore,
$|c_{ij}|=O(\frac1p)$.
Thus, similar to  the blowup analysis in the proof of Lemma \ref{lem3.3},
it follows that
there exists the  constant $C_i$, $i\in J_3\cup J_4$, such that
$$
\hat{\phi}_i(\tilde{z}_i)\to C_i\frac{|\tilde{z}_i|^2-1}{|\tilde{z}_i|^2+1}
\quad\text{uniformly in } C^0_{loc}(\mathbb{R}^2).
$$
From Lebesgue's theorem and the radial properties of  $\omega^{0i}$
and $U^i$, it follows  that for $i\in J_3$,
\begin{gather*}
E_{i1}(\hat{\phi}_i)\to C_i\int_{\mathbb{R}^2}
\frac{32(|z_i|^2-1)\operatorname{Re}(z_i)}
{[1+|z_i|^2]^4}[\omega^{0i}-U^i-\frac{(U^i)^2}2]dz_i=0,\\
E_{i2}(\hat{\phi}_i)\to C_i\int_{\mathbb{R}^2}
\frac{32(|z_i|^2-1)\operatorname{Im}(z_i)}
{[1+|z_i|^2]^4}[\omega^{0i}-U^i-\frac{(U^i)^2}2]dz_i=0,
\end{gather*}
and for $i\in J_4$,
$$
E_{i1}(\hat{\phi}_i)\to C_i\int_{\mathbb{R}_+^2}
\frac{32(|\tilde{z}_i|^2-1)\operatorname{Re}(\tilde{z}_i)}
{[1+|\tilde{z}_i|^2]^4}[\omega^{0i}-U^i-\frac{(U^i)^2}2]d\tilde{z}_i=0,
$$
which together with $\eqref{3.5d}$ implies
$\langle \phi,\,L(\eta_{2i}Z_{ij})\rangle=o(\frac1p)$.
Then by \eqref{3.5b}-\eqref{3.5c}, it implies that
$p(\sum_{i\in J_3\cup J_4}|c_{i1}|
+\sum_{i\in J_3}|c_{i2}|)=o(1)$, which contradicts with the assumption
\eqref{3.5j}, and so
estimate \eqref{3.5} is established. Moreover, by \eqref{3.5e},
it also implies  that
\begin{equation}\label{3.5g}
|c_{ij}|\leq C\|h\|_{*},
\end{equation}
which implies that there exists a unique trivial solution to
problem  \eqref{3.3} with $h\equiv 0$.  Thus, from Fredholm's
alternative, there exists a unique solution $\phi$, scalars
$c_{ij}$, $i\in J_3$, $j=1,2$, and $c_{i1}$, $i\in J_4$,  of problem
\eqref{3.3} for any $h\in \mathcal {C}_{*}$, which completes the proof.
\end{proof}

\begin{remark} \label{rmk3.5}\rm
Given $h\in L^{\infty}(\Omega_\varepsilon)$ with
$\|h\|_*<\infty$, let $\phi$ be the solution to \eqref{3.3} given by 
Proposition \ref{prop3.1}.
Multiplying the first equation in \eqref{3.3} by $\phi$ and integrating by parts,
 we obtain
$$
\|\phi\|_{H^1}^2:=\int_{\Omega_\varepsilon}|\nabla\phi|^2
+\varepsilon_p^2\phi^2=\int_{\Omega_\varepsilon}W_q\phi^2
+\int_{\Omega_\varepsilon}h\phi.
$$
Moreover, using Lemma \ref{lem2.3}, we can prove that
$$
\big|\int_{\Omega_\varepsilon}W_q\phi^2\big|\leq C\|\phi\|_{\infty}^2,
$$
and therefore
$$
\|\phi\|_{H^1}\leq C(\|h\|_*+\|\phi\|_{\infty}).
$$
\end{remark}

Now, we  solve  the intermediate nonlinear problem: for any points
$q\in\Lambda^{\tilde{m}}_{m}(\delta)$,
we find  a function $\phi$,  scalars $c_{ij}$, $i\in J_3$, $j=1,2$, 
and $c_{i1}$, $i\in J_4$, such that
\begin{equation}\label{4.1}
\begin{gathered}
L(\phi)=R_q+N(\phi)+\sum_{i\in J_3\cup J_4}c_{i1}\chi_iZ_{i1}
+\sum_{i\in J_3}c_{i2}\chi_iZ_{i2} \quad
\text{in } \Omega_{\varepsilon},\\
\frac{\partial}{\partial\nu}\phi=0\quad \text{on } \partial\Omega_{\varepsilon},\\
\int_{\Omega_{\varepsilon}}\chi_iZ_{ij}\phi=0 \quad 
\forall i\in J_3,\;j=1,2;\; i\in J_4,\;j=1.
\end{gathered}
\end{equation}

\begin{proposition} \label{prop3.6}
There exist  $C>0$  and $p_0>1$ such that for any $p>p_0$ and
$q\in\Lambda^{\tilde{m}}_{m}(\delta)$,
problem \eqref{4.1} admits a unique solution $\phi\in
L^{\infty}(\Omega_{\varepsilon})$, scalars
 $c_{ij}$, $i\in J_3$, $j=1,2$, and $c_{i1}$, $i\in J_4$, such that
\begin{equation}\label{4.2}
\|\phi\|_{\infty}\leq C/p^3,\quad
\|\phi\|_{H^1}\leq C/p^3. \quad
|c_{ij}|\leq C/p^4.
\end{equation}
\end{proposition}

The proof of the above proposition  can be done along the
lines of those of \cite[Lemma 4.1]{MW1}; we omit it here.


\begin{remark} \label{rmk3.7}\rm
Using the fixed point characterization of the solution $\phi=\phi(q)$ to
\eqref{4.1}, the Implicit Function Theorem and Remark \ref{rmk3.5}, we can easily
 verify  that $\phi(q)$ is differentiable with respect to
$q\in\Lambda^{\tilde{m}}_{m}(\delta)$, in $L^{\infty}(\Omega_\varepsilon)$ 
and $H^1(\Omega_\varepsilon)$.
\end{remark}

\begin{remark} \label{rmk3.8}\rm
The function $V_q+\phi$, with $\phi$ given by Proposition \ref{prop3.6}, 
is positive in $\overline{\Omega}_\varepsilon$. In fact, we  observe first
that $p|\phi|\to0$ uniformly over compacts of $\overline{\Omega}_\varepsilon$.
In addition, from \eqref{2.7c} we argue that, in
the region close to some point $q_i$, $V_q+\phi$ is positive. 
Outside this region, we may conclude the same from
\eqref{2.6a} and \eqref{2.13a}.
\end{remark}

\section{Variational reduction}

After problem \eqref{4.1} has been solved, we find a solution of \eqref{2.23}
with $m+\tilde{m}\geq 1$, and hence for \eqref{a} if
$q\in\Lambda^{\tilde{m}}_{m}(\delta)$
satisfies
\begin{equation}\label{5.1}
c_{ij}(q)=0\quad \forall i\in J_3,\; j=1,2;\; i\in J_4,\;
j=1.
\end{equation}
To solve it we  consider the energy functional of \eqref{a},
\begin{equation}\label{6.1}
J_p(u)=\frac1{2}\int_{\Omega}(|\nabla
u|^2+u^2)dx-\frac1{p+1}\int_{\Omega}S(x)u^{p+1}dx,
\end{equation}
and its finite-dimensional restriction
\begin{equation}\label{6.1aa}
F_p(q)=J_p(U_q+\tilde{\phi})\quad \forall q\in\Lambda^{\tilde{m}}_{m}(\delta),
\end{equation}
where $U_q$ is defined in \eqref{2.6} and
\begin{equation}\label{6.1a}
\tilde{\phi}(q)(x)=\varepsilon_p^{-\frac{2}{p-1}}\phi(q)(\varepsilon_p^{-1}x).
\end{equation}
The following proposition tells us that critical points of $F_p$ 
correspond to solutions of \eqref{5.1}.


\begin{proposition} \label{prop4.1}
The functional $F_p$ is of class $C^1$. Moreover, for $p$ large enough,
if  $D_{q}F_p(q)=0$,  then $q$ satisfies  \eqref{5.1}.
\end{proposition}

\begin{proof}
A direct consequence of the results in Remark \ref{rmk3.7} is the fact that
$F_p(q)$ is a $C^1$-function of $q$ since the map
$q\to\phi$ is a $C^1$-map in $H^1(\Omega_\varepsilon)$.
Define
\begin{equation}\label{6.2}
I_p(v)=\frac1{2}\int_{\Omega_{\varepsilon}}(|\nabla
v|^2+\varepsilon_p^2v^2)dy-\frac1{p+1}\int_{\Omega_{\varepsilon}}
S(\varepsilon_p y)v^{p+1}dy.
\end{equation}
Then, making a change of variable, we have
\begin{equation}\label{6.2a}
\varepsilon_p^{\frac4{p-1}}F_p(q)=I_p(V_q+\phi).
\end{equation}
Since $D_qF_p(q)=0$, we have that
\begin{equation} \label{5.5}
\begin{aligned}
0&=D I_p(V_q+\phi)[D_q V_q+D_q\phi] \\
&=\sum_{i,j}c_{ij}\int_{\Omega_{\varepsilon}}\chi_i Z_{ij}
(D_q V_q+D_q\phi) \\
&=\sum_{i,j}c_{ij}\int_{\Omega_{\varepsilon}}\chi_i Z_{ij}
D_q V_q-\phi D_q[\chi_i Z_{ij}],
\end{aligned}
\end{equation}
because  $\int_{\Omega_{\varepsilon}}\chi_iZ_{ij}\phi=0$.
By the expression  of $V_q$ in \eqref{2.13a}, a direct computation shows that
for any $l\in J_3$, $s=1,2$, and $l\in J_4$, $s=1$,
$$
\partial_{(q_l)_s}V_q=\frac{\frac{1}{\varepsilon_p\mu_l}}{p^{\frac{p}{p-1}}\mu_l^{\frac2{p-1}}
c_l(q_l)^{\frac1{p-1}}}\big\{\frac{4(z_l)_s}
{1+|z_l|^2}-\frac{\partial_{(z_l)_s}\omega^{0l}}{p}
-\frac{\partial_{(z_l)_s}\omega^{1l}}{p^2}\big\}+O(\frac{\varepsilon^\tau_p}p).
$$
Consequently, \eqref{5.5} can be written as,
for each $l\in J_3$, $s=1,2$, and $l\in J_4$, $s=1$,
\begin{equation}
\Big[\frac{\mu_lA_l}{p^{\frac p{p-1}}\mu_l^{\frac2{p-1}}
c_l(q_l)^{\frac1{p-1}}}\int_0^{R_0+1}\chi(r)\frac{16r^{3}}{(\,1+r^2)^2}
dr\Big]c_{ls}+\sum_{i,j}c_{ij}O(\frac1{p^2})=0,
\end{equation}
where $A_l=\pi$ for $l\in J_3$, and
$A_l=\frac12\pi$ for $l\in J_4$.
This is a  strictly diagonal dominant system for $p$ sufficiently large.
We thus get that $c_{ls}=0$ for any $l\in J_3$, $s=1,2$, or $l\in J_4$, $s=1$.
\end{proof}

Next, we need to give the expansion of $F_p$ in terms of 
$\varphi^{\tilde{m}}_{m}$ defined in \eqref{b} as $p$ goes to  $+\infty$.

\begin{proposition} \label{prop4.2}
There exist constants $k_1$, $k_2$ and $k_3>0$ depending
only on the points $q_i$,  $i\in J_1\cup J_2$, such that
\begin{equation}\label{5.3}
F_p(q)=\frac{k_1}{p}-\frac{2k_1}{p^2}\log p
+\frac{k_2}{p^2}-\frac{k_3}{p^2}\varphi^{\tilde{m}}_{m}(q)+O(\frac{\log^2p}{p^3}),
\end{equation}
uniformly for all points $q\in\Lambda_{m}^{\tilde{m}}(\delta)$.
\end{proposition}

\begin{proof}
Multiplying the first equation in \eqref{4.1} by $V_q+\phi$ and integrating 
by parts, we obtain
$$
\int_{\Omega_{\varepsilon}}|\nabla
(V_q+\phi)|^2+\varepsilon_p^2(V_q+\phi)^2
=\int_{\Omega_{\varepsilon}}S(\varepsilon_p y)(V_q+\phi)^{p+1}
+\sum_{i,j}c_{ij}\int_{\Omega_\varepsilon}\chi_iZ_{ij}V_q.
$$
Since $V_q$ is a bounded function, by \eqref{4.2} we obtain that
$$
\int_{\Omega_{\varepsilon}}|\nabla
(V_q+\phi)|^2+\varepsilon_p^2(V_q+\phi)^2
=\int_{\Omega_{\varepsilon}}S(\varepsilon_p y)(V_q+\phi)^{p+1}+O(\frac1{p^4}),
$$
uniformly for $q\in\Lambda_{m}^{\tilde{m}}(\delta)$. Hence, by \eqref{6.2} 
and \eqref{6.2a} we have
\begin{equation}\label{5.4}
F_p(q)=(\frac1{2}-\frac{1}{p+1})\varepsilon_p^{-\frac4{p-1}}
\int_{\Omega_\varepsilon}|\nabla
(V_q+\phi)|^2+\varepsilon_p^2(V_q+\phi)^2+O(\frac1{p^4}).
\end{equation}
We expand the  term $\int_{\Omega_\varepsilon}|\nabla
V_q|^2+\varepsilon_p^2V_q^2$: in view of \eqref{2.7c} and \eqref{2.13c} 
we obtain 
\begin{align*}
&\int_{\Omega_\varepsilon}|\nabla V_q|^2+\varepsilon_p^2V_q^2\\
&=\int_{\Omega_\varepsilon}V_q(-\Delta V_q+\varepsilon_p^2V_q)\\
&=\sum_{i\in\cup_{l=1}^4J_l}\frac{1}{p^{\frac{2p}{p-1}}\mu_i^{\frac4{p-1}}
c_i(q_i)^{\frac2{p-1}}}\int_{|z_i|\leq\delta(v_i\rho_i)^{-1}}|z_i|^{2\alpha_i}\\
&\quad\times\Big\{e^{U^i}+\frac{e^{U^i}\omega^{0i}-f^{0i}}p
 +\frac{e^{U^i}\omega^{1i}-f^{1i}}{p^2}\Big\}
 \big\{p+U^i+\frac{1}p\omega^{0i}+\frac{1}{p^2}\omega^{1i}\big\}dz_i
 +O(\frac1{p^3})\\  
&=\sum_{i\in\cup_{l=1}^4J_l}\frac{A_i}{p^{\frac{2p}{p-1}}\mu_i^{\frac4{p-1}}
 c_i(q_i)^{\frac2{p-1}}}\int_{\mathbb{R}^2}\Big\{p|z_i|^{2\alpha_i}
 e^{U^i}+|z_i|^{2\alpha_i}[U^i-\frac{(U^i)^2}{2}+\omega^{0i}]e^{U^i}\Big\}\\
&\quad +O(\frac1{p^3})\\
&=\sum_{i\in\cup_{l=1}^4J_l}\big\{\frac1p
 [1-\frac{2\log p}{p}-\frac{2}{p}\log c_i(q_i)]d_i
 -\frac4{p^2}d_i\log\mu_i+\frac1{p^2}A_ie_i\big\}
 +O(\frac{\log^2p}{p^3}),
\end{align*}
where $A_i=1$ for $i\in J_1\cup J_3$, $A_i=\frac12$ for $i\in J_2\cup J_4$, and
the last equality is due to the following relations:
\begin{gather*}
p^{-\frac{2p}{p-1}}=\frac1{p^2}-\frac{2}{p^3}\log p+O(\frac{\log^2p}{p^4}),\\
\mu_i^{-\frac4{p-1}}=1-\frac4p\log\mu_i+O(\frac1{p^2}),\\
c_i(q_i)^{-\frac{2}{p-1}}=1-\frac{2}{p}\log c_i(q_i)+O(\frac1{p^2}),\\
e_i=\int_{\mathbb{R}^2}|z_i|^{2\alpha_i}[U^i-\frac12(U^i)^2+\omega^{0i}]e^{U^i}
\quad \forall i\in\cup_{l=1}^4 J_l.
\end{gather*}
From the expansion  of $\mu_i$ in  \eqref{2.6bb}, we have 
\begin{equation}  \label{5.2}
\begin{aligned}
&\int_{\Omega_\varepsilon}|\nabla V_q|^2+\varepsilon_p^2V_q^2 \\
&=\sum_{i\in\cup_{l=1}^{4}J_l}\Big\{(1-\frac{2\log p}p
 +\frac3p)\frac{d_i}p+\frac{A_ie_i}{p^2}-\frac{d_i}{p^2}\
  \Big[2\log c_i(q_i)\\
&\quad +d_i H(q_i,q_i)+\sum_{j\neq i}d_j G(q_i,q_j)\Big]\Big\}
  +O(\frac{\log^2p}{p^3})\\
&=-\frac{1}{p^2}\varphi^{\tilde{m}}_{m}(q)
 +\sum_{i\in\cup_{l=1}^{4}J_l}\big\{(1-\frac{2\log p}p+\frac3p)
 \frac{d_i}p+\frac{A_ie_i}{p^2}\big\} \\
&\quad -\sum_{i\in J_1\cup J_2}\frac{d_i}{p^2}\Big\{2\log c_i(q_i)
+d_iH(q_i,q_i)+\sum_{j\in J_1\cup J_2,\,j\neq i}d_jG(q_i,q_j)\Big\}
+O(\frac{\log^2p}{p^3}),
\end{aligned}
\end{equation}
uniformly for $q\in\Lambda_{m}^{\tilde{m}}(\delta)$. In particular,
\begin{equation}\label{5.2a}
\|V_q\|_{H^1}^2=\int_{\Omega_\varepsilon}|\nabla
V_q|^2+\varepsilon_p^2V_q^2=O(\frac1p).
\end{equation}
Furthermore, by \eqref{4.2} and \eqref{5.2a}, we obtain
\begin{equation}\label{5.2aa}
2\int_{\Omega_\varepsilon}[\nabla
V_q\nabla\phi+\varepsilon_p^2V_q\phi]+\int_{\Omega_\varepsilon}[|\nabla
\phi|^2+\varepsilon_p^2\phi^2]=O(\frac1{p^{7/2}}).
\end{equation}
Also
\begin{equation}\label{5.6}
\varepsilon_p^{-\frac4{p-1}}=e^{\frac{p}{p-1}}=e+\frac{e}p+O(\frac1{p^2}).
\end{equation}
Thus, inserting \eqref{5.2},  \eqref{5.2aa} and \eqref{5.6} in \eqref{5.4},
 we obtain that  \eqref{5.3} holds.
\end{proof}

\begin{proof}[Proof of Theorem \ref{thm1.2}]
First of all, from Proposition  \ref{prop4.1}, we
can provide a solution to problem \eqref{a} if we adjust
$q\in\Lambda_{m}^{\tilde{m}}(\delta)$ so that it is
a critical point of $F_p(q)$ defined by \eqref{6.1aa}.
This is equivalent to finding a
critical point of
$$
\tilde{F}_p(q):=\frac1{k_3}\left(k_1p-2k_1\log p+k_2-p^2F_p(q)\right),
$$
for suitable constants $k_1$, $k_2$ and $k_3$. On the other hand, from
Proposition \ref{prop4.2}, we have 
\begin{equation}\label{r4}
\tilde{F}_p(q)=\varphi^{\tilde{m}}_{m}(q)+O(\frac{\log^2 p}{p}),
\end{equation}
uniformly for all points $q\in\Lambda_{m}^{\tilde{m}}(\delta)$ as 
$p\to\infty$, where $\varphi^{\tilde{m}}_{m}$ is given by \eqref{b}.

Next, as in \cite[Lemma 6.1]{MW1}, we  have
\begin{equation}\label{6.1b}
\min_{q\in\partial\Lambda_{m}^{\tilde{m}}(\delta)}\varphi_{m}^{\tilde{m}}(q)
\to +\infty \quad\text{as }\delta\to0.
\end{equation}
Thus,  for $\delta$ small enough, $\varphi_{m}^{\tilde{m}}$ has a global
 minimum $M$ in  $\Lambda_{m}^{\tilde{m}}(\delta)$.
This, together with \eqref{r4}, implies that $\tilde{F}_p(q)$ has also
a global minimum point
$q^p\in\Lambda_{m}^{\tilde{m}}(\delta)$ such that
$\varphi_{m}^{\tilde{m}}(q^p)\to M$ as $p\to\infty$.
Moreover,  up to a subsequence, there exists
a global minimum point
$\tilde{q}$ of $\varphi_{m}^{\tilde{m}}$ in  $\Lambda^{\tilde{m}}_{m}(\delta)$
such that  $q^p\to\tilde{q}$ as $p\to\infty$.
The function $u_p=U_{q^p}+\tilde{\phi}(q^p)$, where $\tilde{\phi}(q^p)$ 
is defined in \eqref{6.1a},
is therefore a  solution to \eqref{a} with the
qualitative properties stated in the theorem.
\end{proof}

\subsection*{Acknowledgments}
This research was supported by the National Natural Science 
Foundation of China (No. 11171214).


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