1. Introduction
In this paper, we consider the following fractional problem
where $\bar {\nu }\in {{\mathfrak R}}$, $s\in (0,1)$, $\Omega \subset {{\mathfrak R}}^{N}\,(N> 2s)$ is a bounded domain with smooth boundary and $\varphi _{1}$ is the first positive eigenfunction of the fractional Laplace under the condition $u=0$ in ${{\mathfrak R}}^{N}\setminus \Omega$. $g(t)$ has superlinear growth and satisfies
Here $\alpha =+\infty$ and $\beta =-\infty$ are allowed. For any $\Omega \subset {{\mathfrak R}}^{N}$ and $u\in C_{0}^{\infty }(\Omega )$, we have $u=0$ in ${{\mathfrak R}}^{N}\backslash \Omega$. The fractional Laplace operator $(-\Delta )^{s}$ is defined as follows:
where $P.V.$ stands for the principle value and $C_{N,s}$ is a normalization constant (see for instance [Reference Nezza, Palatucci and Valdinoci14]).
In particular, if $s=1$, equation (1.1) reduces to
Equation (1.2) has been studied first by Ambrosetti et al. in [Reference Ambrosetti and Prodi2], and many results were obtained there, the readers can refer to [Reference Dancer and Yan5–Reference Dancer and Yan7, Reference Lazer and McKenna10–Reference Li, Yan and Yang12, Reference Wei and Yan22]. It is well known (e.g. [Reference Ambrosetti and Prodi2]) that the location of $\alpha$, $\beta$ with respect to the spectrum of $(-\Delta , H_{0}^{1}(\Omega ))$ has great influence on the number of solutions to equation (1.2). Let $0<\Lambda _{1}<\Lambda _{2}\leq \Lambda _{3} \leq \cdots \leq \Lambda _{i}\leq \cdots$ be the eigenvalues of Laplace $-\Delta$ in $H_0^{1}(\Omega )$. In [Reference Lazer and McKenna10] Lazer and McKenna made a conjecture that equation (1.2) has an unbounded number of solutions as $\bar {\nu }\to +\infty$ if $\alpha =+\infty$, $\beta <\Lambda _{1}$, and $g(t)$ does not grow too rapidly.
There were several works related to the Lazer-McKenna conjecture. Breuer et al. [Reference Breuer, McKenna and Plum3] used numerical method to show that equation (1.2) has at least four solutions if $g(t)=t^{2}$ and $\Omega$ is a unit square in ${{\mathfrak R}}^{2}$. Dancer et al. [Reference Dancer and Yan5] proved the Lazer-McKenna conjecture if $g(t)=|t|^{p}$, where $p\in (1,(N+2)/(N-2))$ and $N\geq 3$. Moreover, it is shown in [Reference Dancer and Yan6] that the Lazer-McKenna conjecture is also true if $g(t)=t_{+}^{p}+\lambda t$, where $u_{+}=\max (u,0)$, $N\geq 3$, $p\in (1,(N+2)/(N-2))$, $\lambda <\Lambda _{1}$ or $\lambda \in (\Lambda _{i},\Lambda _{i+1})$ for $i\geq 1$. Later on, Li et al. [Reference Li, Yan and Yang11, Reference Li, Yan and Yang12] and Wei et al. [Reference Wei and Yan22] proved the Lazer-McKenna conjecture if $g(t)=t_{+}^{2^{*}-1}+\lambda t$, where $N\geq 6$, $2^{*}=(2N)/(N-2)$ and $\lambda \in (0,\Lambda _{1})$ or $\lambda \in (\Lambda _{i},\Lambda _{i+1})$ for $i\geq 1$. Recently, in [Reference Abdellaoui, Dieb and Mahmoudi1], Abdellaoui et al. extended the results in [Reference Dancer and Yan5] to fractional Laplace and proved the fractional version of conjecture. This inspires us to consider problem (1.1). Our goal in this paper is to prove the fractional version of the Lazer-McKenna conjecture, extending the results in [Reference Li, Yan and Yang12]. More precisely, we consider the following equation
where $\lambda \in {{\mathfrak R}}$, $2^{*}_{s}=({2N}/{N-2s}),\,N>2s$.
Let $\lambda _{1}<\lambda _{2}\leq \lambda _{3}\leq \cdots \leq \lambda _{i}\leq \cdots$ be the eigenvalues of fractional Laplace $(-\Delta )^{s}$ under the condition $u=0$ in ${{\mathfrak R}}^{N}\setminus \Omega$. Indeed, it follows from [Reference Servadei and Valdinoci20] that
where $X_{0}^{s}(\Omega )$ is given by
with the norm
Furthermore, by [Reference Servadei and Valdinoci20], $\lambda _{1}$ is simple and $\varphi _{1}>0$ in $\Omega$.
Throughout this paper, we always assume that $\lambda$ and $\bar {\nu }$ satisfy one of the following conditions:
($C_{1}$) $\lambda \in (0,\lambda _{1})$ and $\bar {\nu }>0$;
($C_{2}$) $\lambda \in (\lambda _{i},\lambda _{i+1})$ for some $i\geq 1$ and $\bar {\nu }<0$.
The main result in this paper can be stated as follows:
Theorem 1.1 Suppose that $0< s<1$, ($C_{1}$) or ($C_{2}$) is satisfied. Then the number of the solutions for equation (1.3) tends to infinity as $|\bar {\nu }|\to +\infty$ if $N> 6s$.
Obviously, $-({\bar {\nu }}/{\lambda _{1}-\lambda })\varphi _{1}$ is a negative solution of equation (1.3). We will construct solutions of equation (1.3) redin the form
Then $v$ solves
where $\nu =({\bar {\nu }}/{\lambda _{1}-\lambda })$. Thus $\nu \to +\infty$ as $|\bar {\nu }|\to +\infty$.
In the sequel, we mainly consider equation (1.4). We will use Lyapunov-Schmidt reduction method to construct peak solutions of equation (1.4). This method has been widely used to study elliptic problems, see for examples [Reference Peng and Wang15–Reference Peng, Wang and Yan18, Reference Wei and Yan24] and the references therein. The advantage of this method is that we can not only prove the existence of many solutions but also obtain the profile of these solutions. Without loss of generality, we always assume that $\underset {y\in \Omega }{\max }\varphi _{1}(y)=1$ and we denote $S=\{ z\in \Omega : \varphi _{1}(z)=1\}$.
It is well known that
with
solves equation
where $x_{j}\in {{\mathfrak R}}^{N}$ and $\mu _{j}\in (0,\infty )$. In order to simplify notations, we denote $U=U_{0,1}$. Furthermore, in [Reference Dávila, del Pino and Sire8], it is shown that $U$ is non-degenerate, in the sense that, if $\phi$ solves the linearized equation of equation (1.5)
then $\phi$ is a linear combination of
Let $PU_{x_{j},\mu _{j}}$ be the solution of
We will choose $PU_{x_{j},\mu _{j}}$ as a building block of approximate solution. Moreover, we have
Theorem 1.2 Let $k>0$ be an integer and $N> 6s$. Then there exists $\nu _{k}>0$ such that for any $\nu \geq \nu _{k}$, equation (1.4) has a solution of the form
satisfying that as $\nu \to \infty$,
(i) $\phi _{\nu ,k}\in X_{0}^{s}(\Omega )$ and $\|\phi _{\nu ,k}\|\to 0$;
(ii) $\mu _{\nu ,j}\nu ^{-2/(N-6s)}\to t_{0}>0$;
(iii) $\nu ^{2/(N-6s)} |x_{\nu ,i}-x_{\nu ,j}|\to +\infty$ for $i\neq j$;
(iv) $x_{\nu ,j}\to x_{j}^{*}\in \Omega$ with $x_{j}^{*}\in S$;
where the constant $t_{0}$ is defined in (2.1).
In order to expand energy (see appendix B), we have to estimate
If $s=1$, then $\Psi _{x_{j},\mu _{j}}$ solves
Using comparison principle, we can easily obtain the leading term of $\Psi _{x_{j},\mu _{j}}$, for much details, the reader can see [Reference Rey19]. In order to overcome these difficulties due to the fractional Laplace, considering that many mathematics applied $s$-harmonic extension method (see [Reference Caffarelli and Silvestre4]) and studied a new local problem
we turn to obtain the leading term of $\Psi _{x_{j},\mu _{j}}$ by convolution formula of Green function with $U_{x_{j},\mu _{j}}^{2^{*}_{s}-1}$. This idea is mainly from [Reference Dávila, López Rios and Sire9, Reference Long, Yan and Yang13]. For much details, the readers can see appendix A. On the other hand, in order to solve critical points of $K(x,\mu )$ (see § 3), we will use a type of gradient flow method (see [Reference Wei and Yan22, Reference Wei and Yan23]). Indeed, we cannot prove the existence of critical points of $K(x,\mu )$ by using maximization procedure as in [Reference Dancer and Yan5, Reference Dancer and Yan6]. Furthermore, in [Reference Li, Yan and Yang12], Li et al. proved that $K(x,\mu )$ has a saddle point such that $K(x,\mu )$ attained the minimum at $\mu _{i}$ direction and attained maximum at $x_{i}$ direction. Compared with [Reference Li, Yan and Yang12], the gradient flow method we used in this paper will simply be the procedure very much to obtain critical points.
To end this section, we introduce some notations. We define $H^{s}({{\mathfrak R}}^{N})$ the classical Sobolev space
with the norm
We also define $D^{s,2}({{\mathfrak R}}^{N})$ as follows
with the norm
We recall that $X_{0}^{s}(\Omega )$ is a Hilbert space with the product
By [Reference Nezza, Palatucci and Valdinoci14], we can see that
where the constant $C_{N,s}$ is given by
We can also refer to [Reference Servadei and Valdinoci20, Reference Servadei and Valdinoci21] for more properties of $X_{0}^{s}(\Omega )$.
Our paper is organized as follows. In § 2, we will carry out the reduction procedure. Then, we will study the reduced finite dimensional problem and prove theorem 1.2 in § 3. Our notations are standard. We will use $C$ to denote different positive constant from line to line.
2. Finite dimensional reduction
Define
where $x_{j}\in \Omega$, $j=1,\ldots , k$, $x=(x_{1},\ldots ,x_{k})$, $\mu =(\mu _{1},\ldots ,\mu _{k})$, $\tau$ is a small constant, $L$ is a fixed large positive constant and $t_{0}$ is given by
Here the positive constants $A_{2}$ and $A_{3}$ are defined in lemma B.1. Let
Then, for $(x,\mu )\in D_{k,\nu }$, we have
We set
where $x_{j}=(x_{j1},\ldots ,x_{jN})\in {{\mathfrak R}}^{N}$, $j=1,\ldots ,k$, $l=1,\ldots ,N$.
Define the energy functional corresponding to equation (1.4) as follows
Let
Then we expand $J_{\nu }(x,\mu ,\phi )$ at $\phi =0$ as follows
where
and
Now we estimate $l_{\nu }(\phi )$, $Q_{\nu }(\phi ,\psi )$ and $R_{\nu }(\phi )$ respectively.
Lemma 2.1 For any $\phi \in X_{0}^{s}(\Omega )$, we have
Proof. Rewrite $l_{\nu }(\phi )$ as follows:
Note that
where $\sigma >0$ is a small constant. Then we have
Define $\Omega _{j}=\{ z: \mu _{j}^{-1}z+x_{j}\in \Omega \}$, we choose $\sigma >0$ small enough such that
Then
By lemma A.2, we have
the second inequality is because of
In fact, let $R>0$ be such that $\Omega \subset B_{R}(x_j)$, we have $\Omega _j\subset B_{\mu _jR}(0)$. Thus,
By Hölder inequality, we have
the second inequality is because of
In fact, define
For all $y\in \tilde {\Omega }_1$, we have
Hence, we have
Similarly, we have
Combining (2.5)–(2.8) with lemma A.2, we can obtain that
On the other hand,
the last inequality follows from $({2N(N-2s)}/{N+2s})>N$ since $N>6s$.
Lemma 2.2 For any $\phi ,\psi \in X_{0}^{s}(\Omega )$, there exists constant $C>0$ such that
where $C$ is independent of $\nu$.
Proof. Using Hölder inequality, we can easily check this conclusion.
It follows from lemma 2.2 that $Q_{\nu }(\phi ,\psi )$ is a bounded bi-linear functional in $X_{0}^{s}(\Omega )$. Then there exists a bounded linear operator $Q_{\nu }$ from $E_{x,\mu ,k}$ to $E_{x,\mu ,k}$ such that
Now, we intend to prove that operator $Q_{\nu }$ is invertible in $E_{x,\mu ,k}$.
Proposition 2.3 There exists constant $\rho >0$, independent of $\nu$ and $(x,\mu )\in D_{k,\nu }$, such that
Proof. We argue by contradiction. Assume that there exist $\nu _{n}\to \infty$, $(x_{n},\mu _{n})\in D_{\nu _{n},k}$, $x_{j,n}\to x_{j}^{*}\in S$ and $\phi _{n}\in E_{x_{n},\mu _{n},k}$ such that
Without loss of generality, we may assume that $\|\phi _{n}\|=1$. Let $\tilde {\phi }_{i,n}(y)=\mu _{i,n}^{-(N-2s)/2}\phi _{n}(\mu _{i,n}^{-1}y+x_{i,n})$, $\Omega _{i,n}\,{=}\,\{y: \mu _{i,n}^{-1}y+x_{i,n}\in \Omega \}$. Then $\|\tilde {\phi }_{i,n}\|\,{=}\,\|\phi _{n}\|\,{=}\,1$. Thus, we may assume that there exists $\tilde {\phi }_{i}\in D^{s,2}({{\mathfrak R}}^{N})$ such that
We claim that $\tilde {\phi }_{i}$ solves
In fact, it is sufficient to show that
Since
we have
where $\tilde {\eta }(y)=\eta (\mu _{i,n}^{-1}y+x_{i,n})$, $\tilde {U}_{j,n}=\mu _{i,n}^{-(N-2s)/2}PU_{x_{j,n},\mu _{j,n}}(\mu _{i,n}^{-1}y+x_{i,n})$,
where $l=1,\ldots ,N$, $j=1,\ldots ,k$ and $\tilde {V}_{j,l,n}$, $\tilde {V}_{j,n}$ are given by
For any $\eta \in C_{0}^{\infty }({{\mathfrak R}}^{N})$, we can choose $a_{j,l,n}$ and $b_{j,n}$ such that
Noting that $\eta$ has compact support and the support of $\tilde {V}_{j,l,n}$ and $\tilde {V}_{j,n}$ moves to infinity as $n\to \infty$ if $i\neq j$. Thus, we can see that $a_{j,l,n}\to 0$ and $b_{j,n}\to 0$ if $i\neq j$. Furthermore, we can check that $a_{i,l,n}$ and $b_{i,n}$ are bounded. Since $(x_{n},\mu _{n})\in D_{\nu _{n},k}$, then $\nu _{n}\mu _{i,n}^{-(N-2s)/2}\to 0$. Substituting $\tilde {\eta }$ in (2.15) and letting $n\to \infty$, we derive that
where $a_{i,l}=\underset {n\to \infty }{\lim }a_{i,l,n}$ and $b_{i}=\underset {n\to \infty }{\lim }b_{i,n}$. On the other hand,
and
Thus, (2.13) follows from (2.16)–(2.18). Therefore, we have proved this claim.
We recall that $U$ is non-degenerate, that is, if $\tilde {\phi }_{i}$ solves (2.12), then there exists some constants $\bar {c}_{l}$ and $\bar {c}$ such that
Note that $\phi _{n}\in E_{x_{n},\mu _{n},k}$, then $\tilde {\phi }_{i,n}\in \tilde {E}_{x_{n},\mu _{n},k}$. So we can obtain that
and
which imply that $\tilde {\phi }_{i}=0$. Then for any $R>0$,
Moreover, we have
Thus,
where $o_{R}(1)\to 0$ as $R\to \infty$. Combining (2.14) with (2.20), we deduce that
Note that $\phi _{n}\in X_{0}^{s}(\Omega )$ and $\|\phi _{n}\|=1$. We may assume that there exits $\phi \in X_{0}^{s}(\Omega )$ such that
We claim that $\phi =0$. Indeed, for any $\eta \in C_{0}^{\infty }(\Omega )$, we choose $c_{j,l,n}$ such that
In order to estimate $c_{j,l,n}$ and $d_{j,n}$, multiplying (2.21) by $\frac {\partial PU_{x_{i,n},\mu _{i,n}}}{\partial x_{ih}}$ and $\frac {\partial PU_{x_{i,n},\mu _{i,n}}}{\partial \mu _{i}}$ respectively, we have
and
Note that
and
Combining (2.22) with (2.24), we see that $c_{j,l,n}=O(\mu _{j}^{-1}\mu _{j}^{-(N-2s)/2})$. By (2.23) and (2.25), we obtain that $d_{j,n}=O(\mu _{j}\mu _{j}^{-(N-2s)/2})$. Thus,
the last inequality follows from $({2N(N-2s)}/{N+2s})>N$ since $N>6s$. Using the similar computation, we also have
Inserting $\bar {\eta }$ into (2.21), combining (2.26) with (2.27) and letting $n\to \infty$, we can deduce that
Since $\lambda \neq \lambda _{i}$, $\phi =0$. Hence, the claim is completed.
Taking $\eta =\phi _{n}$ in (2.21), we derive that
which contradicts with $\|\phi _{n}\|=1$.
Lemma 2.4 For any $\phi \in X_{0}^{s}(\Omega )$, it holds
Proof. Using the fact that for $a,b>0$,
we can easily check this conclusion. Here, we omit it.
Proposition 2.5 There exists $\nu _{k}>0$ such that for $\nu \geq \nu _{k}$, there exists a $C^{1}$-map $\phi _{\nu ,x,\mu }: D_{k,\nu }\to X_{0}^{s}(\Omega )$, such that $\phi _{\nu ,x,\mu }\in E_{x,\mu ,k}$ satisfies
Furthermore,
where $\sigma$ is a small positive constant.
Proof. Set
First, by lemma 2.1, we see that $l_{\nu }(\phi )$ is a bounded linear functional in $E_{x,\mu ,k}$. Then, there exists $l_{\nu }$ such that
Combining this with (2.11), we can obtain that (2.29) is equivalent to
It follows from proposition 2.3 that $Q_{\nu }$ is invertible in $E_{x,\mu ,k}$ and
Thus, (2.30) can be written as
Now, we prove that $\mathcal {A}$ is a contraction map from $\mathcal {N}_{x,\mu ,k}$ to $\mathcal {N}_{x,\mu ,k}$.
On one hand, for any $\phi _{1}$, $\phi _{2}\in \mathcal {N}_{x,\mu ,k}$, using lemma 2.4, we have
if $\nu$ is large enough. Hence, $\mathcal {A}$ is a contraction map.
On the other hand, for any $\phi \in \mathcal {N}_{x,\mu ,k}$, applying lemma 2.1 and lemma 2.4 again, we have
if $\nu$ is large enough. Therefore, $\mathcal {A}$ is a contraction map from $\mathcal {N}_{x,\mu ,k}$ to $\mathcal {N}_{x,\mu ,k}$. By contraction mapping theorem, there exists a unique $\phi _{\nu ,x,\mu }\in \mathcal {N}_{x,\mu ,k}$ such that (2.31) holds. Moreover,
3. Proof of main result
In this section, we will choose suitable $(x,\mu )\in D_{k,\nu }$ such that
is a solution of equation (1.4). We define
where $\phi _{\nu ,x,\mu }$ is obtained in proposition 2.5. Using proposition 2.5 and lemma B.2, we deduce that
where the positive constants $A_{1}$, $A_{2}$, $A_{3}$ $A(x_{i},x_{j})$ are defined in lemma B.2 and $\sigma >0$ is a small constant.
Now, we intend to estimate the derivative of $K(x,\mu )$. It follows from proposition 2.5 that there exist constants $c_{ih}$, $d_{i}$, $i=1,\ldots ,k$, $h=1,\ldots ,N$ such that
Thus
Hence, we have to estimate $({\partial J_{\nu }(x,\mu ,\phi _{\nu ,x,\mu })}/{\partial \mu _{j})}$, $c_{ih}$ and $d_{i}$.
Lemma 3.1 Let $\phi _{\nu ,x,\mu }$ be obtained in proposition 2.5. Then
and
where $\sigma >0$ is a small constant, constants $A_{2}$, $A_{3}$ are defined in lemma B.1.
Proof. By a direct computation, we have
It follows from proposition 2.5 and (2.10) that
Note that
Then, using lemma A.2, proposition 2.5 and Hölder inequality, we obtain that
On the other hand, by a similar computation in (B.7), we can obtain
Lemma 3.2 Let $c_{jl}$ and $d_{j}$ be defined in (3.2). Then
and
Proof. Multiplying $({\partial PU_{x_{j},\mu _{j}}}/{\partial \mu _{j})}$ and $({\partial PU_{x_{j},\mu _{j}}}/{\partial x_{jl})}$ by (3.2), respectively, we obtain
and
On the other hand, by a direct computation, we have
and
Combining (3.10)–(3.13) with lemma 3.1, we can complete the proof.
Based on lemma 3.1 and lemma 3.2, we can conclude the following conclusion.
Proposition 3.3 Let $(x,\mu )\in D_{k,\nu }$. Then
where $\sigma >0$ is a small constant.
Define
Then it is easy to check that $f(t)$ has unique minimum point
on $(0,\infty )$. Let
where $\eta >0$ is a small fixed constant. Denote
Consider the following flow
We have
Proposition 3.4 Let $N>6s$. Then the flow does not leave $D_{k,\nu }$ before it reaches $K^{\alpha _{1}}$.
Proof. Denote
Suppose that $\mu _{j}=(t_{0}+L\nu ^{-s\tau })\nu ^{2/(N-6s)}$ for some $j$. Then by (3.14), we have
if we choose $L>0$ is large.
Similarly, if $\mu _{j}=(t_{0}-L\nu ^{-s\tau })\nu ^{2/(N-6s)}$ for some $j$. Then by (3.14), we have
So the flow does not leave $D_{k,\nu }$.
Now, we suppose that $|x_{i}-x_{j}|^{N-2s}= \nu ^{-(2N-8s)/(N-6s)+s\tau }$. Then we have
Thus, applying (3.1), we can derive
where the last equality follows from the fact that $f(t_{j})=f(t_{0})+O(|t-t_{j}|^{2})$.
On the other hand, if $|\varphi _{1}(x_{j})-1|= \nu ^{-s\tau }$, then using (3.1), we can obtain
Thus, we complete the proof.
Proof of theorem 1.2 We will prove that $K(x,\mu )$ has a critical point in $D_{k,\nu }$. Define
where $h_1(x,\mu )=x$ if $x\in \partial D_{k,\nu }^{1}$. Here we denote $D^{1}_{k,\nu }=\{x: (x,\mu )\in D_{k,\nu }\}$ and define the boundary of $D^{1}_{k,\nu }$ by $\partial D_{\nu ,k}^{1}$. Furthermore, we denote $D^{2}_{k,\nu }=\{\mu : (x,\mu )\in D_{k,\nu }\}$.
Let
We claim that $c_{\nu }$ is a critical value of $K$. In order to prove this claim, it is sufficient to prove that
(i) $\alpha _{1}< c_{\nu }<\alpha _{2}$,
(ii) $\underset {(x,\mu )\in \partial D_{\nu ,k}^{1}\times D_{\nu ,k}^{2}}{\sup }K(h(x,\mu ))<\alpha _{1}$, $\forall \, h\in \Gamma$.
Obviously, (ii) directly follows from (3.15) and (3.16).
Now, we prove (i). Using (3.1), we can easily check that $c_{\nu }<\alpha _{2}$.
For any $h=(h_{1},h_{2})\in \Gamma$, by the definition of $h$, we have ${h}_{1}(x,\mu )=x$ if $x \in \partial D_{\nu ,k}^{1}$. Define
Then $\tilde {h}_{1}(x)=x$ for any $x \in \partial D_{\nu ,k}^{1}$. Thus, by degree argument, we can obtain
Hence, for any $\xi \in D_{\nu ,k}^{1}$, there exists $\tilde {x}\in D_{\nu ,k}^{1}$ such that
Let $\tilde {\mu }=h_{2}(\tilde {x},t_{0}\nu ^{-2/(N-6s)})$. Then we have
Choose $\xi _{j}\in \Omega$ such that $dist(\xi _{j},S)\leq \nu ^{-s\tau }$ and $|\xi _{i}-\xi _{j}|\geq c_{1}\nu ^{-s\tau }$, where $c_{1}$ is a small positive constant. By a direct computation, we have
Combining (3.1) with (3.17), we obtain
Consequently, we complete the proof.
Appendix A. Basic estimate
In this section, we always suppose that $dist(x_{j},\partial \Omega )\geq \delta >0$, where $\delta$ is a small constant. Let $G(y,z)$ be the Green's function of $(-\Delta )^{s}$ in $\Omega$. That is, $G$ satisfies
where $\delta _{y}$ denotes the Dirac mass at the point $y$. The regular part of $G$ is given by
where $\Gamma (y,z)$ is given by
Let
Then we have
Lemma A.1 It holds
Proof. By proposition 2.4 in [Reference Long, Yan and Yang13], we can see that $G(y,z)\geq 0$ and $H(y,z)\geq 0$. Then
and
Lemma A.2 We have
where $j=1,\ldots ,k$, $i=1,\ldots ,N$ and $c_{0}=\int _{{{\mathfrak R}}^{N}}U^{2^{*}_{s}-1}$.
Proof. Note that
and
Then, we have
the last equality follows from (B.3), where $\Omega _{j}=\{z : \mu _{j}^{-1}z+x_{j}\in \Omega \}$. By a similar argument above, we can prove (A.2) and (A.3).
Appendix B. Energy expand
In this section, we will expand $J_{\nu }(x,\mu ,0)$ and its derivatives. First, we recall that the energy function corresponding to equation (1.4) is given by
Lemma B.1 We have
where $\sigma$ is a small positive constant and $A_{1}$, $A_{2}$, $A_{3}$ are defined by
Proof. By a direct computation, we have
Let $R>0$ such that $\Omega \subset B_{R}(x_{j})$. Choose $\sigma$ small such that $N+2s-\sigma (N-2s)>N$. Using the following estimate
we find
the last equality is due to the following estimate
Lemma B.2 We have
where $A_{2}$, $A_{3}$ are defined in lemma B.1, $\sigma$ is a small positive constant and $A(x_{i},x_{j})$ is defined by
Proof. By a direct computation, we have
Noting that for $i\neq j$, we have
and
Now we estimate the last term in (B.4). By a similar computation as (B.2), we obtain that
Lemma B.3 We have
where $A_{2}$, $A_{3}$ are defined in lemma B.1 and $\sigma >0$ is a small constant.
Proof. By a direct computation, we have
Using the similar computation, we can conclude the following result.
Lemma B.4 We have
Acknowledgments
The authors would like to express their gratitude to the reviewers for careful reading and helpful suggestions which led to an improvement of the original manuscript. This research was supported by the National Natural Science Foundation of China (No.11831009; No.12071169).