Hostname: page-component-586b7cd67f-l7hp2 Total loading time: 0 Render date: 2024-11-21T18:50:56.701Z Has data issue: true hasContentIssue false

ASYMPTOTIC BEHAVIOUR OF THE LEAST ENERGY SOLUTIONS TO FRACTIONAL NEUMANN PROBLEMS

Published online by Cambridge University Press:  13 September 2024

SOMNATH GANDAL
Affiliation:
Indian Institute of Technology Gandhinagar Palaj, Gnadhinagar, Gujarat 382055, India e-mail: [email protected]
JAGMOHAN TYAGI*
Affiliation:
Indian Institute of Technology Gandhinagar Palaj, Gandhinagar, Gujarat 382055, India e-mail: [email protected]
Rights & Permissions [Opens in a new window]

Abstract

We study the asymptotic behaviour of the least energy solutions to the following class of nonlocal Neumann problems:

$$ \begin{align*} \begin{cases} { d(-\Delta)^{s}u+ u= \vert u\vert^{p-1}u } & \text{in } \Omega, \\ {u>0} & \text{in } \Omega, \\ { \mathcal{N}_{s}u=0 } & \text{in } \mathbb{R}^{n}\setminus \overline{\Omega}, \end{cases} \end{align*} $$

where $\Omega \subset \mathbb {R}^{n}$ is a bounded domain of class $C^{1,1}$, $1<p<({n+s})/({n-s}),\,n>\max \{1, 2s \}, 0<s<1, d>0$ and $\mathcal {N}_{s}u$ is the nonlocal Neumann derivative. We show that for small $d,$ the least energy solutions $u_d$ of the above problem achieve an $L^{\infty }$-bound independent of $d.$ Using this together with suitable $L^{r}$-estimates on $u_d,$ we show that the least energy solution $u_d$ achieves a maximum on the boundary of $\Omega $ for d sufficiently small.

Type
Research Article
Copyright
© The Author(s), 2024. Published by Cambridge University Press on behalf of Australian Mathematical Publishing Association Inc.

1. Introduction

We discuss the asymptotic behaviour of nonconstant least energy solutions of the following problem:

(1-1) $$ \begin{align}\begin{cases} { d(-\Delta)^{s}u+ u= \vert u\vert^{p-1}u } &\text{in } \Omega, \\ {u>0} &\text{in } \Omega, \\ { \mathcal{N}_{s}u=0 } & \text{in } \mathcal{C} \overline{\Omega}, \end{cases}\end{align} $$

where $\Omega \subset \mathbb {R}^{n}$ is a bounded domain of class $C^{1,1},\,\,1<p<({n+s})/({n-s}), n>\max \{1, 2s \}, 0<s<1, d>0,\, \mathcal {C} \Omega := \mathbb {R}^n\setminus \Omega $ and $\mathcal {N}_{s}u$ is the nonlocal Neumann derivative, which is defined next. The nonlocal operator $(-\Delta )^{s}$ is called the fractional Laplacian, which is defined for smooth functions as follows:

(1-2) $$ \begin{align} (-\Delta)^{s}u(x)= c_{n,s}\,\mathrm{PV}\int_{\mathbb{R}^{n}}\frac{u(x)-u(y)}{\vert x-y\vert^{n+2s}}\,dy. \end{align} $$

Here, by PV, we mean the Cauchy principal value and $c_{n,s}$ is a normalising constant, given by

$$ \begin{align*} c_{n,s}=\bigg(\int_{\mathbb{R}^{n}} \frac{1-\text{cosx}_{1}}{\vert x\vert^{n+2s}}\,dx\bigg)^{-1}; \end{align*} $$

see for instance [Reference Di Nezza, Palatucci and Valdinoci12] for the details. Recently, Dipierro et al. [Reference Dipierro, Ros-Oton and Valdinoci14] have introduced a new nonlocal Neumann condition $\mathcal {N}_{s}, $ which is defined as follows:

$$ \begin{align*} \mathcal{N}_{s}u(x):=c_{n,s}\int_{\Omega}\frac{u(x)-u(y)}{\vert x-y\vert^{n+2s}}\,dy, \quad x \in \mathcal{C} \overline{\Omega}. \end{align*} $$

The advantage of this nonlocal Neumann condition is that it has simple probabilistic interpretation and (1-1) has a variational structure. Further, it naturally arises from the superposition of Brownian and Lévy processes; see [Reference Dipierro and Valdinoci16] for the details. We recall that $ \mathcal {N}_{s}u$ approaches the classical Neumann derivative $\partial _{\nu }u$ as s goes to $1.$

In the last few decades, mathematical analysis of biological phenomena has gained much attention. For example, chemotaxis models, which are also known as Keller–Segel models [Reference Keller and Segel28], have been widely studied in different directions in many papers; see [Reference Arumugam and Tyagi3, Reference Horstmann24, Reference Horstmann25] for a survey on this subject. Chemotaxis refers to the movement of cells or organisms in response to chemical gradients in their environment. The analysis on the steady-state for a chemotactic aggregation model with linear or logarithmic sensitivity function was thoroughly done in many papers; see for instance [Reference Kabeya and Ni27, Reference Lin, Ni and Takagi31, Reference Ni and Takagi35].

Let us point out that the following semilinear Neumann problem is an example of the Keller–Segel model with a logarithmic chemotactic sensitivity:

(1-3) $$ \begin{align}\begin{cases} {-d \Delta u+ u= \vert u\vert^{p-1}u } &\text{in } \Omega, \\ {u>0} &\text{in } \Omega, \\[3pt] {\dfrac{\partial u}{\partial \nu}=0 } &\text{on } \partial \Omega, \end{cases} \end{align} $$

where $d>0$ , $\Omega \subset \mathbb {R}^n$ is a bounded domain with smooth boundary and $1<p \leq ({n+2})/({n-2})$ if $n \geq 3$ and $1<p<\infty $ if $p=2$ ; see [Reference Lin, Ni and Takagi31] for the details. Problem (1-3) admits a nonconstant solution for d sufficiently small; see [Reference Adimurthi and Mancini1, Reference Lin, Ni, Hildebrandt, Kinderlehrer and Miranda30, Reference Lin, Ni and Takagi31]. Lin et al. [Reference Lin, Ni and Takagi31] and Lin and Ni [Reference Lin, Ni, Hildebrandt, Kinderlehrer and Miranda30] established the existence of solutions to (1-3) in the subcritical case $1<p < ({n+2})/({n-2}) .$ In the critical case, when $ p= ({n+2})/({n-2}),$ Adimurthi and Mancini [Reference Adimurthi and Mancini1] obtained a solution of (1-3). There have been developments on the asymptotic behaviour of solutions to such equations. In the subcritical case, $1<p < ({n+2})/({n-2}),$ Ni and Takagi [Reference Ni, Takagi, Lloyd, Ni, Peletier and Serrin34, Reference Ni and Takagi35] have studied the shape of the least energy solutions of (1-3). They have shown that the least energy solutions tend to zero as the diffusion constant d goes to zero except at a finite number of points. Moreover, the maximum of a solution $u_{d}$ of (1-3) is attained at a unique point on the boundary of $\Omega .$ The critical case was examined by Adimurthi et al. [Reference Adimurthi, Pacella and Yadava2] using blow-up analysis. We refer to [Reference He, Rădulescu and Zou23] for the existence, nonexistence and the asymptotic behaviour of solutions to fractional Choquard equations with local perturbations.

We mention that Problem (1-1), which we explore in this paper is a nonlocal analogue of the classical problem (1-3).

The substitution of standard diffusion with fractional diffusion is a perceived approach in modelling feeding procedures across a wide range of organisms. In many situations observed in nature, Lévy flights are often used as an accomplished search strategy by living organisms [Reference Bartumeus, Peters, Pueyo, Marrasé and Catalan5, Reference Levandowsky, White and Schuste29]. Since the fractional Laplacian $(-\Delta )^{s}$ is an infinitesimal generator of a Lévy process, dispersal is better modelled by the nonlocal operator $(-\Delta )^{s}$ . The generalised Keller–Segel model with nonlocal diffusion term $d(-\Delta )^{s}$ , where d is a positive constant is used to investigate chemotaxis with anomalous diffusion. For the fractional Keller–Segel model, we refer to [Reference Escudero18, Reference Huang and Liu26]. In [Reference Huang and Liu26], Huang and Liu studied the existence, stability, uniqueness and regularity of solutions for the following model in dimension $n \geq 2$ :

$$ \begin{align*} \begin{cases} u_{t}= d(-\Delta)^{s} u- \nabla \cdot (u \nabla \phi ), & x \in \mathbb{R}^n, \,\,\,t \geq 0, \\ -\Delta \phi=u, & \\ u(x,0)=u_{0}(x), \end{cases} \end{align*} $$

where d is a positive constant, $u(t, x)$ is the density of some biological cells and $\phi (t, x)$ is the chemical substance concentration. We mention the work [Reference Choi, Kim and Lee9], where the authors have investigated the asymptotic behaviour of solutions for nonlinear elliptic problems for fractional Laplacians with Dirichlet boundary conditions. We refer to [Reference Dipierro, Soave and Valdinoci15] for the regularity, monotonicity and other results on fractional equations in Lipschitz sets, [Reference Gandal and Tyagi22] for the existence of solutions to critical Neumann problems and [Reference Molica Bisci, Rădulescu and Servadei32] for an in-depth treatment of variational methods to nonlocal fractional problems.

Motivated by the above literature, the works on the fractional Laplacian [Reference Mugnai, Perera and Proietti Lippi33, Reference Ros-Oton and Serra36, Reference Servadei and Valdinoci38, Reference Servadei and Valdinoci39] and the very recent works on the nonlocal Neumann problem for fractional Laplacians and its connections with fractional Keller–Segel models, we have the following natural question to ask.

Question. Can we establish the asymptotic behaviour of the least energy solutions of (1-1)?

The aim of this paper is to answer the above question. More precisely, we discuss the asymptotic behaviour of the least energy solutions of (1-1).

A weak solution of (1-1) can be obtained as a critical point of the following energy functional $J_{d}$ :

$$ \begin{align*} J_{d}(u):=\frac{1}{2} \bigg[ \frac{dc_{n,s}}{2} \int_{T(\Omega)} \frac{\vert u(x)-u(y)\vert^{2}}{\vert x-y\vert^{n+2s}}\,dx\,dy + \int_{\Omega}u^{2}\,dx \bigg] -\frac{1}{p+1}\int_{\Omega}{\lvert u \rvert}^{p+1}\,dx, \quad u \in H_{\Omega}^{s}. \end{align*} $$

In the above equation, $T(\Omega )= \mathbb {R}^{2n}\setminus (\mathcal {C} \Omega )^{2}$ and the space $H_{\Omega }^{s}$ is defined in (2-1). The functional $J_{d}$ is well defined and of class $C^2$ by Theorem 2.1, stated next. An application of the Mountain-Pass lemma applied to the functional $J_{d}$ yields that

(1-4) $$ \begin{align} c_{d}:=\inf_{\gamma \in \Gamma}\max_{[0,1]}J_{d}(\gamma(t)) \end{align} $$

is a critical value of $J_{d}.$ In the above equation, by $\Gamma ,$ we mean the following set:

$$ \begin{align*} \Gamma = \{\gamma \in C([0,1]; H^{s}_{\Omega}) \mid \gamma(0)=1, \, \gamma(1)=u \}, \end{align*} $$

where $u \in H^{s}_{\Omega }$ , and $u>0$ satisfies $J_{d}(u)=0.$ It turns out that $c_d$ is the least positive critical value; see Lemma 3.3. For the details, one may refer to [Reference Barrios, Montoro, Peral and Soria4, Theorem 6.1] and [Reference Chen7, Theorem 1.1], where the authors have obtained a nonnegative weak solution $u_{d}$ of (1-1) with critical value $c_{d}$ , provided d is sufficiently small. Moreover, $u_{d}$ satisfies

$$ \begin{align*}0< J_{d}(u_{d}) \leq C d^{{n}/{2s}},\end{align*} $$

where the constant C is independent of $d.$ Consequently, $u_{d}$ is nonconstant. From the proof of [Reference Chen7, Theorem 1.1], it is immediate to see that the critical points of $J_{d}$ are not sign-changing in $\Omega $ . In fact, when $u_{d} \leq 0,$ we can choose $-u_{d}$ to have a nonnegative solution of (1-1). By the strong maximum principle (see [Reference Cinti and Colasuonno10, Theorem 2.6]), one can see that $u_{d}>0$ almost everywhere (a.e.) in $\Omega .$ Further, since $u_{d}$ satisfies the Neumann condition, $\mathcal {N}_{s}u_{d}(x)=0$ in $\mathcal {C} \Omega $ , which implies that $u_{d}>0$ a.e. in $\mathbb {R}^{n}.$

Definition 1.1. We call a critical point $u_{d}$ of $J_{d}$ with $J_{d}(u_{d})=c_{d}$ the least energy solution or Mountain-Pass solution of (1-1).

We show the asymptotic behaviour of the least energy solutions of (1-1) following a similar approach to that of Ni and Takagi [Reference Ni and Takagi35] for (1-3). They used a positive solution w of the nonlinear Schrödinger equation

$$ \begin{align*}- \Delta u + u= \vert u\vert^{p-1}u \text{ in } \mathbb{R}^{n}, \quad 1<p< \frac{n+2}{n-2}\end{align*} $$

to study the asymptotic behaviour of the least energy solutions of (1-3). The fractional nonlinear Schrödinger equation

(1-5) $$ \begin{align} (-\Delta)^{s}u + u = \vert u\vert^{p-1}u \quad\text{in } \mathbb{R}^{n}, \end{align} $$

where $1<p<({n+2s})/({n-2s}), n>\max \{1, 2s\},\,0<s<1$ , is thoroughly studied; see for instance [Reference Chen and Gao8, Reference Dipierro, Palatucci and Valdinoci13, Reference Felmer and Quaas20, Reference Felmer and Wang21] and the references therein.

Let us discuss the main idea of this work, which goes as follows.

Let $c_{d}$ be the critical value of $J_{d},$ which is defined in (1-4). Following the arguments of [Reference Ni and Takagi35], we use a positive solution w of (1-5) to observe the asymptotic behaviour of $c_{d}$ as $d\downarrow 0.$ More specifically, w is used to build a suitable function $\phi _d$ to compare $c_d$ with $\max _{t\geq 0} J_{d}(t \phi _{d}).$ In particular, we obtain an inequality

$$ \begin{align*} c_{d}< \frac{d^{{n}/{2s}}}{2}F(w) \end{align*} $$

for d sufficiently small, where F is the functional associated with (1-5), defined in (2-2). This is closely related to the location of the maximum point of a solution $u_{d}$ of (1-1) on the boundary of $\Omega .$

Now, we summarise the above discussion in terms of the following three main theorems. A priori, it is known that for $1 \leq p < ({n+s})/({n-s}),$ any weak solution u of (1-1) satisfies

$$ \begin{align*} \Vert u\Vert_{L^{\infty}(\Omega)} \leq K, \end{align*} $$

where $K>0$ is some constant depending on $\Omega , p$ and d; see [Reference Mugnai, Perera and Proietti Lippi33, Theorem 3.1]. In the next result, we obtain a bound for the least energy solution $u_{d}$ of (1-1), which is independent of $d.$

Theorem 1.2. Let $u_{d}$ be the least energy solution of (1-1). Then

(1-6) $$ \begin{align} d \frac{c_{n,s}}{2} \int_{T(\Omega)} \frac{\vert u_{d}(x)-u_{d}(y)\vert^{2}}{\vert x-y\vert^{n+2s}}\,dx\,dy + \int_{\Omega}u_{d}^{2}\,dx=& \int_{\Omega} u_{d}^{p+1}\,dx \leq C_{0}d^{{n}/{2s}}, \end{align} $$

where $C_{0}>0$ is some constant depending on $p.$ Moreover, there is a constant $C_{1}>0$ depending only on p and $\Omega $ such that

$$ \begin{align*} \sup_{\Omega}u_{d}(x)\leq C_{1}. \end{align*} $$

In the next theorem, we show that the $L^r$ -norm of the least energy solution $u_d$ is bounded by $d^{{n}/{2s}}$ times some constant independent of $d.$

Theorem 1.3. Let $u_{d}$ be the least energy solution of (1-1). Then

(1-7) $$ \begin{align} b(r)d^{{n}/{2s}}\leq \int_{\Omega} u_{d}^{r}\,dx \leq B(r)d^{{n}/{2s}} \quad \text{if } 1\leq r \leq \infty, \end{align} $$
(1-8) $$ \begin{align} b(r)d^{{n}/{2s}}\leq \int_{\Omega} u_{d}^{r}\,dx \leq B(r)d^{{nr}/{2s}} \quad \text{if } 0<r<1, \end{align} $$

where $b(r)$ and $B(r)$ are positive constants such that $b(r)<B(r)$ and are independent of $d.$

We show the asymptotic behaviour in the next theorem.

Theorem 1.4. Let $\Omega \subset \mathbb {R}^n$ be a bounded domain of class $C^{1,1}.$ Let $u_{d}$ be the least energy solution of (1-1). If $u_{d}$ achieves a maximum at a point $z_{d} \in \overline {\Omega },$ then for all d sufficiently small, we have $z_{d} \in \partial \Omega .$

The plan of the paper is as follows. In Section 2, we recollect known results that are useful for our analysis. In Section 3, we study the regularity of the least energy solution of (1-1) and complete the proof of Theorem 1.2. In Section 4, we derive $L^{r}$ -estimates for the least energy solutions of (1-1). Section 5 contains the proof of Theorem 1.4. The proof of inequality (3-8) is a part of Appendix A.

2. Auxiliary results

Let us recall some important results that are used in this paper.

Theorem 2.1 (Fractional Sobolev embedding [Reference Di Nezza, Palatucci and Valdinoci12])

Let $n>2s$ and $2_{s}^{*}={2n}/({n-2s})$ be the fractional critical exponent. Then, we have the following inclusions.

  1. (1) For any function $u\in C_{0}(\mathbb {R}^{n})$ and for $q\in [0, 2_{s}^{*}-1],$

    $$ \begin{align*} \Vert u\Vert_{L^{q+1}(\mathbb{R}^{n})}^{2} \leq B(n,s)\int_{\mathbb{R}^{n}}\int_{\mathbb{R}^{n}} \frac{\vert u(x)-u(y)\vert^{2}}{\vert x-y\vert^{n+2s}}\,dx\,dy \end{align*} $$
    for some positive constant $B.$ That means $H^{s}(\mathbb {R}^{n})$ is continuously embedded in $L^{q+1}(\mathbb {R}^{n}).$
  2. (2) Let $\Omega \subset \mathbb {R}^{n}$ be a bounded extension domain for $H^{s}(\Omega ).$ Then, the space $H^{s}(\Omega )$ is continuously embedded in $L^{q+1}(\Omega )$ for any $q\in [0, 2_{s}^{*}-1],$ that is,

    $$ \begin{align*} \Vert u\Vert_{L^{q+1}(\Omega)}^{2} \leq B(n,s,\Omega)\Vert u\Vert_{H^{s}(\Omega)}^{2}\end{align*} $$
    for some positive constant $B.$ Further, the above embedding is compact for any $q\in [0, 2_{s}^{*}-1).$

Let $T(\Omega ):=\mathbb {R}^{2n}\setminus (\mathbb {R}^{n}\setminus \Omega )^{2}$ be a cross-shaped set on a bounded domain $\Omega \subset \mathbb {R}^n$ . Define

(2-1) $$ \begin{align} H_{\Omega}^{s}:=\{ u: \mathbb{R}^{n}\longrightarrow \mathbb{R} \text{ measurable}: {\Vert u\Vert}_{H_{\Omega}^{s}}< \infty \}, \end{align} $$

which is equipped with the norm

$$ \begin{align*} \Vert u\Vert_{H_{\Omega}^{s}}:=\bigg(\Vert u\Vert_{L^{2} (\Omega)}^{2}+\int_{T(\Omega)}\frac{{\lvert u(x)-u(y)\rvert}^{2}}{{\lvert x-y \rvert}^{n+2s}}\,dx\,dy \bigg)^{{1}/{2}}. \end{align*} $$

Remark 2.2. Here, $H_{\Omega }^{s}$ is a Hilbert space (see [Reference Dipierro, Ros-Oton and Valdinoci14, Proposition 3.1]).

Let us define the following set:

$$ \begin{align*}\mathcal{L}_{s}:= \bigg\{u: \mathbb{R}^{n}\longrightarrow \mathbb{R} \text{ measurable}: \int_{\mathbb{R}^n} \frac{\vert u(x)\vert}{1+\vert x\vert^{n+2s}}\,dx < \infty \bigg\}.\end{align*} $$

The condition $u \in \mathcal {L}_{s}$ is useful to give a sense to the pointwise definition of fractional Laplacians (1-2).

Lemma 2.3 [Reference Cinti and Colasuonno10, Lemma 2.3]

Let $\Omega \subset \mathbb {R}^n$ be a bounded set. Then, $H^{s}_{\Omega } \subset \mathcal {L}_{s}.$

Next, we recall a few known results about the fractional Schrödinger equation (1-5).

Definition 2.4. A measurable function $u: \mathbb {R}^{n} \longrightarrow \mathbb {R}$ is called a weak solution of (1-5) if it satisfies the following equation:

$$ \begin{align*} & \frac{c_{n,s}}{2} \int_{\mathbb{R}^{n}}\int_{\mathbb{R}^{n}} \frac{(u(x)-u(y))(\psi(x)-\psi(y))}{\vert x-y\vert^{n+2s}}\,dx\,dy\\ &\quad + \int_{\mathbb{R}^{n}}u(x)\psi(x)\,dx = \int_{\mathbb{R}^{n}} \vert u(x)\vert^{p-1}u(x)\psi(x)\,dx \end{align*} $$

for all $\psi \in C_{0}^{1}(\mathbb {R}^{n}).$

We define the corresponding energy functional $F: H^{s}(\mathbb {R}^n) \longrightarrow \mathbb {R} $ as follows:

(2-2) $$ \begin{align} F(u):=\frac{1}{2} \bigg[ \frac{c_{n,s}}{2} \int_{\mathbb{R}^{n}}\int_{\mathbb{R}^{n}} \frac{\vert u(x)-u(y)\vert^{2}}{\vert x-y\vert^{n+2s}}\,dx\,dy + \int_{\mathbb{R}^{n}}u^{2}\,dx \bigg] -\frac{1}{p+1}\int_{\mathbb{R}^{n}}|u|^{p+1}\,dx. \end{align} $$

The weak solutions of (1-5) correspond to the critical points of $F.$

Definition 2.5. A function $u \in \mathcal {L}_{s}(\mathbb {R}^{n}) \cap C^{2s+\epsilon }(\mathbb {R}^n),$ when $0<s<\tfrac 12$ , $2s+\epsilon <1$ , or $u \in C^{1, 2s+\epsilon -1}(\mathbb {R}^n) \cap \mathcal {L}_{s}(\mathbb {R}^{n}),$ when $\tfrac 12\leq s<1$ , $2s+\epsilon -1<1 $ , is said to be a classical solution of (1-5) if it satisfies (1-5) pointwise in $\mathbb {R}^{n}.$

The next result gives us a positive, radially symmetric solution of (1-5), which decays at infinity.

Theorem 2.6 [Reference Felmer and Quaas20, Theorem 3.4]

Let u be the weak solution of (1-5). Then, $u \in L^{q}(\mathbb {R}^{n}) \cap C^{\alpha }(\mathbb {R}^{n})$ for some $q \in [2, \infty ) $ and $\alpha \in (0,1).$ Moreover,

$$ \begin{align*} \lim_{\vert x\vert \rightarrow \infty}u(x)=0. \end{align*} $$

Theorem 2.7 [Reference Felmer and Quaas20, Theorem 1.3]

Equation (1-5) has a weak solution in $H^{s}(\mathbb {R}^{n}),$ which satisfies $u \geq 0$ a.e. in $\mathbb {R}^{n}.$ Moreover, u is a classical solution, which satisfies $u>0$ in $\mathbb {R}^{n}.$

The following theorem shows that the solutions of (1-5) have a power type of decay at infinity.

Theorem 2.8 [Reference Felmer and Quaas20, Theorem 1.5]

Let u be a positive classical solution of (1-5) such that

$$ \begin{align*}\lim_{\vert x\vert \rightarrow \infty}u(x)=0.\end{align*} $$

Then, there exist constants $0< C_{1} \leq C_{2}$ such that

$$ \begin{align*} \frac{C_{1}}{\vert x\vert^{n+2s}}\leq u(x) \leq \frac{C_{2}}{\vert x\vert^{n+2s}} \quad \text{for all } \vert x\vert\geq 1. \end{align*} $$

One can see that there exist some $m>0$ and $s_{0}>0$ such that for $f(u)=u^{p}-u,$

$$ \begin{align*} \frac{f(v)-f(u)}{v-u}\leq \frac{v^{p}-u^{p}}{v-u}\leq C (v+u)^{m} \quad\text{for all } 0 < u< v < s_{0}, \end{align*} $$

where $C>0$ is some constant. Also, it is simple to see that $f: [0,\infty ) \to \mathbb {R}$ is locally Lipschitz. Consequently, we have the following result on the radial symmetry and monotonicity property of positive solutions of (1-5).

Theorem 2.9 [Reference Felmer and Wang21, Theorem 1.2]

Let u be a positive classical solution of (1-5) such that

$$ \begin{align*}\lim_{\vert x\vert \rightarrow \infty}u(x)=0.\end{align*} $$

Further, assume that there exists

$$ \begin{align*}t> \max \bigg\{\frac{2s}{m}, \frac{n}{m+2} \bigg\}\end{align*} $$

such that u satisfies $u(x)=O({1}/{\vert x\vert ^{t}})$ as $ \vert x\vert \rightarrow \infty .$ Then, u is radially symmetric and strictly decreasing about some point in $\mathbb {R}^{n}.$

Remark 2.10. Since

$$ \begin{align*} \frac{C_{1}}{\vert x\vert^{n+2s}}\leq u(x) \leq \frac{C_{2}}{\vert x\vert^{n+2s}} \quad \text{for all } \vert x\vert\geq 1, \end{align*} $$

we can take $t=n+2s$ in the above theorem.

Now, [Reference Secchi37, Proposition 4.1] ascertains that if $u \in \mathbb {R}^n$ is a weak solution of (1-5), then u satisfies the following Pohozaev identity:

$$ \begin{align*} \mathcal{P}(u):= \frac{(n-2s)c_{n,s}}{4}\int_{\mathbb{R}^n} \int_{\mathbb{R}^n} \frac{\vert u(x)-u(y)\vert^2}{\vert x-y\vert^{n+2s}}\,dx\,dy + \frac{n}{2}\int_{\mathbb{R}^n} u^2 \,dx-\frac{n}{p+1} \int_{\mathbb{R}^n} u^{p+1}=0. \end{align*} $$

Let us define

$$ \begin{align*} \mathcal{G}:=\{ u \in H^s(\mathbb{R}^n) \setminus \{0\} \mid \mathcal{P}(u)=0 \}. \end{align*} $$

In [Reference Chen and Gao8], the authors have obtained a weak solution $w \in H^{s}(\mathbb {R}^{n})$ of (1-5) with the least energy among all other solutions. In particular, they have proved the following result.

Theorem 2.11 [Reference Chen and Gao8, Theorem 1.2]

Equation (1-5) has a weak solution $w \in H^s(\mathbb {R}^n)$ such that

$$ \begin{align*}0<F(w)=\inf_{u \in \mathcal{G}}F(u) .\end{align*} $$

Combining Theorems 2.7, 2.8, 2.9 and 2.11, we have the following result.

Theorem 2.12. Equation (1-5) has a positive classical solution $w \in H^{s}(\mathbb {R}^n)$ satisfying:

  1. (a) w has a power type of decay at infinity, that is, there exist constants $0< C_{1} \leq C_{2}$ such that

    $$ \begin{align*} \frac{C_{1}}{\vert x\vert^{n+2s}}\leq w(x) \leq \frac{C_{2}}{\vert x\vert^{n+2s}} \quad \text{for all } \vert x\vert\geq 1; \end{align*} $$
  2. (b) w is radially symmetric, that is, $w(x)=w(r)$ with $r=\vert x\vert ;$

  3. (c) for any nonnegative classical solution $u \in H^{s}(\mathbb {R}^{n})$ of (1-5), $0<F(w) \leq F(u)$ holds unless $u=0.$

Definition 2.13. We call $w,$ given by Theorem 2.12, a ground state solution of (1-5).

3. Regularity and bounds for the least energy solution $u_{d}$

Let $s\in (0,1)$ and $\Omega \subset \mathbb {R}^{n}$ be a bounded domain of class $C^{1,1}.$

Definition 3.1. A measurable function $u: \mathbb {R}^{n} \longrightarrow \mathbb {R}$ is said to be a weak solution of (1-1) if it satisfies the following equation:

(3-1) $$ \begin{align} &\frac{dc_{n,s}}{2} \int_{T(\Omega)} \frac{(u(x)-u(y))(\psi (x)-\psi(y))}{\vert x-y\vert^{n+2s}}\,dx\,dy\nonumber\\ &\quad+ \int_{\Omega}u(x)\psi(x)\,dx=\int_{\Omega} \vert u(x)\vert^{p-1}u(x)\psi(x)\,dx \end{align} $$

for all $\psi \in H_{\Omega }^{s}.$

We have the following result on the existence of a weak solution of (1-1).

Theorem 3.2 ([Reference Barrios, Montoro, Peral and Soria4, Theorem 6.1], [Reference Chen7, Theorem 1.1])

There exists a nonnegative weak solution $u_{d}$ of (1-1) with critical value $c_{d}$ , provided d is sufficiently small. Moreover, $u_{d}$ satisfies

$$ \begin{align*}0< J_{d}(u_{d}) \leq C d^{{n}/{2s}},\end{align*} $$

where the constant C is independent of $d.$ Consequently, $u_{d}$ is nonconstant.

Define

$$ \begin{align*}M[v]:=\sup_{t \geq 0}J_{d}(tv), \quad v\in H_{\Omega}^{s}.\end{align*} $$

In the next lemma, we indicate a useful characterisation of the critical value $c_{d}.$ We follow similar lines of proof to [Reference Ni and Takagi35, Lemma 3.1].

Lemma 3.3. The critical value $c_{d}$ is independent of the choice of $u \in H_{\Omega }^{s}$ such that $u \geq 0,~u \not \equiv 0$ and $J_{d}(u)=0.$ In fact, $c_{d}$ is the least positive critical value of $J_{d},$ which is given by

(3-2) $$ \begin{align} c_{d}=\inf\{M[v] \mid v\in H_{\Omega}^{s},~v\not \equiv 0, v\geq 0 \text{ in } \Omega \}. \end{align} $$

Proof. For $v\in H_{\Omega }^{s},$ let

$$ \begin{align*}\Omega^{+}=\{x \in \Omega \mid v(x)>0\}.\end{align*} $$

Now, for all those v satisfying $\vert \Omega ^{+}\vert>0,$ define

$$ \begin{align*}g_{d}(t):=J_{d}(tv) \quad \text{for } t \geq 0. \end{align*} $$

First, we show that $g_{d}(t)$ has a unique maximum. For this,

$$ \begin{align*} g^{\prime}_{d}(t)= t\bigg[ \frac{dc_{n,s}}{2} \int_{T(\Omega)} \frac{\vert v(x)-v(y)\vert^{2}}{\vert x-y\vert^{n+2s}}\,dx\,dy + \int_{\Omega}v^{2}\,dx \bigg] -t^{p}\int_{\Omega}{v }^{p+1}\,dx. \end{align*} $$

Therefore, $g^{\prime }_{d}(t_{0})=0$ for some $t_{0}>0$ if and only if

$$ \begin{align*}\frac{dc_{n,s}}{2} \int_{T(\Omega)} \frac{\vert v(x)-v(y)\vert^{2}}{\vert x-y\vert^{n+2s}}\,dx\,dy + \int_{\Omega}v^{2}\,dx = t_{0}^{p-1}\int_{\Omega} v^{p+1}\,dx.\end{align*} $$

Note that the right-hand side is strictly increasing in $t_{0}.$ And hence there exists a unique $t_{0}>0$ such that $g^{\prime }_{d}(t_{0})=0.$ Since $g_{d}(t)>0$ for $t>0$ small and $g_{d}(t) \rightarrow -\infty $ as $t \rightarrow +\infty ,$ one easily find that $g_{d}(t)$ has a unique maximum.

Let us fix a function $u \not \equiv 0, u\geq 0$ in $H_{\Omega }^{s} $ with $J_{d}(u)=0.$ Let $u_{d}$ be a positive solution of (1-1) obtained by applying the Mountain-Pass lemma and $c_{d}$ the corresponding critical value. We have $J_{d}(u_{d})=c_{d}$ and $J_{d}^{'}(u_{d})=0.$ Since $u_{d}>0$ and $J_{d}^{'}(u_{d})=0,$

(3-3) $$ \begin{align} M[u_{d}]=c_{d}, \end{align} $$

and hence

(3-4) $$ \begin{align} c_{d}\geq \inf\{M[v] \mid v\in H_{\Omega}^{s},~v\not \equiv 0, v\geq 0 \text{ in } \Omega \}. \end{align} $$

In contrast, assume that strict inequality occurs in (3-4). Then,

$$ \begin{align*}M[v_{0}]<c_{d},\end{align*} $$

for some $v_{0} \geq 0,\, v_{0} \not \equiv 0 $ in $H_{\Omega }^{s}. $ Therefore, there exists some $t_{1}>0$ such that $t_{1}v_{0}=u_{0}$ satisfies $J_{d}(u_{0})=0.$ Denote by U the subspace of $H_{\Omega }^{s}$ spanned by u and $u_{0}.$ Consider the subset of U defined as follows:

$$ \begin{align*}U^{+}:=\{ \alpha u + \beta u_{0}\mid \alpha,~\beta \geq 0 \}.\end{align*} $$

Suppose S is a circle on U of radius R so large that $R> \max \{ \Vert u\Vert , \Vert u_{0}\Vert \}$ and $J_{d}\leq 0$ on $S \cap U^{+}.$ Assume that $\gamma $ is the path made up of the line segment with endpoints $0$ and ${Ru_{0}}/{\Vert u_{0}\Vert },$ the circular arc $ S\cap U^{+}$ and the line segment with endpoints ${Ru}/{\Vert u\Vert }$ and $u.$ One can easily see that, along $\gamma $ , $J_{d}$ is positive only on the line segment joining $0$ and $u_{0}.$ Hence,

$$ \begin{align*} \max_{v \in \gamma}J_{d}(v)=M[v_{0}] < c_{d},\end{align*} $$

which is a contradiction to (1-4). Thus, we have equality in (3-4), that is,

$$ \begin{align*} c_{d}= \inf\{M[v] \mid v\in H_{\Omega}^{s},~v\not \equiv 0, v\geq 0 \text{ in } \Omega \}. \end{align*} $$

Note that $J_{d}(v)=J_{d}(-v)$ for any $v \in H^{s}_{\Omega }$ . Since any nontrivial critical point of $J_{d}$ is either positive or negative a.e. in $\Omega ,$ from the above discussion, one can see that $c_{d}$ is the least positive critical value of $J_{d}$ . This completes the proof.

The following lemma gives us the regularity estimate. A similar result is already proved in [Reference Cinti and Colasuonno10, Lemma 3.6] and [Reference Cinti and Colasuonno11, Remark 4.9].

Lemma 3.4. Let $u \in H_{\Omega }^{s}$ be a weak solution of (1-1). Let $u \in L^{\infty }(\Omega ),$ then $u \in L^{\infty }(\mathbb {R}^{n}).$ Moreover:

  1. (1) for $0<s<\tfrac 12$ , $u \in C^{2}(\Omega )$ if $p>3-2s$ and $u \in C^{1, p-2+2s}(\Omega )$ if $2<p\leq 3-2s;$

  2. (2) for $\tfrac 12 \leq s< 1$ , $u \in C^{2}(\Omega ).$

Now, we prove that the least energy solution $u_{d}$ is bounded by some constant independent of $d.$

Proof of Theorem 1.2

The proof of the first inequality of Theorem 1.2 is fairly standard and simple, and can be seen in the literature; for instance, see [Reference Chen and Gao8, Theorem 1.1]. Since it is short, for the sake of completeness, we include it here. For this,

$$ \begin{align*} J_{d}(u_{d}):=\frac{1}{2} \bigg[ \frac{c_{n,s}d}{2} \int_{T(\Omega)} \frac{\vert u_{d}(x)-u_{d}(y)\vert^{2}}{\vert x-y\vert^{n+2s}}\,dx\,dy + \int_{\Omega}u^{2}\,dx \bigg] -\frac{1}{p+1}\int_{\Omega}u_{d}^{p+1}\,dx. \end{align*} $$

Since $u_{d}$ is a critical point of $J_{d}$ ,

$$ \begin{align*} J_{d}^{\prime}(u_{d})=0 \quad\text{on } H_{\Omega}^{s}. \end{align*} $$

This implies that

(3-5) $$ \begin{align} d\frac{c_{n,s}}{2} \int_{T(\Omega)} \frac{\vert u_{d}(x)-u_{d}(y)\vert^{2}}{\vert x-y\vert^{n+2s}}\,dx\,dy + \int_{\Omega}u_{d}^{2}\,dx =\int_{\Omega}u_{d}^{p+1}\,dx. \end{align} $$

Hence, from the above equations,

(3-6) $$ \begin{align} J_{d}(u_{d})&= \bigg(\frac{1}{2}-\frac{1}{p+1}\bigg)\int_{\Omega}u_{d}^{p+1}\,dx \\&= \frac{(p-1)}{2(p+1)} \int_{\Omega}u_{d}^{p+1}\,dx.\nonumber \end{align} $$

Now, by Theorem 3.2, we have $J_{d}(u_{d})\leq C d^{{n}/{2s}}$ , where the constant C depends only on $p.$ Using this inequality in the above equation,

$$ \begin{align*} \int_{\Omega}u_{d}^{p+1}\,dx \leq \frac{2(p+1)}{p-1}Cd^{{n}/{2s}}. \end{align*} $$

Taking $C_{0}={2(p+1)}/({p-1})C$ proves the first inequality of Theorem 1.2. The proof of the second inequality of Theorem 1.2 is a little constructive. We claim that

$$ \begin{align*}\displaystyle \sup_{\Omega}u_{d}(x) \leq C_{1}\end{align*} $$

for some constant $C_{1}>0$ depending on p and $\Omega $ only. Multiplying (1-1) by $u_{d}^{2t-1}$ and integrating over $\Omega ,$

(3-7) $$ \begin{align} \frac{c_{n,s}d}{2}\int_{T(\Omega)} \frac{(u_{d}(x)-u_{d}(y))(u_{d}^{2t-1}(x)-u_{d}^{2t-1}(y))}{\vert x-y\vert^{n+2s}}\,dx\,dy + \int_{\Omega}u_{d}^{2t}\,dx = \int_{\Omega}u_{d}^{p+2t-1}\,dx. \end{align} $$

Now, we use the following inequality. We give the proof of this inequality in the Appendix. Let $x, y \geq 0$ be real numbers and $k\geq 1$ , then

(3-8) $$ \begin{align} \frac{1}{k}(x^{k}-y^{k})^{2}\leq (x-y)(x^{2k-1}-y^{2k-1}). \end{align} $$

Consequently,

(3-9) $$ \begin{align} \frac{1}{t}\int_{T(\Omega)} \frac{(u_{d}^{t}(x)-u_{d}^{t}(y))^{2}}{\vert x-y\vert^{n+2s}}\,dx\,dy \leq \int_{T(\Omega)} \frac{(u_{d}(x)-u_{d}(y))(u_{d}^{2t-1}(x)-u_{d}^{2t-1}(y))}{\vert x-y\vert^{n+2s}}\,dx\,dy. \end{align} $$

From (3-7) and (3-9),

(3-10) $$ \begin{align} \frac{dc_{n,s}}{2t}\int_{T(\Omega)} \frac{(u_{d}^{t}(x)-u_{d}^{t}(y))^{2}}{\vert x-y\vert^{n+2s}}\,dx\,dy + \int_{\Omega}u_{d}^{2t}\,dx \leq \int_{\Omega}u_{d}^{p+2t-1}\,dx. \end{align} $$

Further, by the fractional Sobolev embedding (Theorem 2.1),

(3-11) $$ \begin{align} \bigg(\int_{\Omega}{\vert v\vert^{2_{s}^{*}}} \bigg)^{2/2_{s}^{*}} \leq \frac{A}{d}\bigg(d\frac{c_{n,s}}{2}\int_{\Omega}\int_{\Omega} \frac{\vert v(x)-v(y)\vert^{2}}{\vert x-y\vert^{n+2s}}\,dx\,dy + \int_{\Omega}\vert v\vert^{2}\,dx \bigg), \end{align} $$

where $d\in (0,d_{0})$ for some $d_{0}>0$ , $A>0$ some constant, $v\in H^{s}(\Omega )$ and $2_{s}^{*}={2n}/({n-2s}).$ The embedding constant A depends only on n, s, $d_{0}$ and $\Omega .$ To see this, let us define

$$ \begin{align*} \Omega_{d}:=\bigg \{ y : \frac{y}{d^{1/2s}} \in \Omega \bigg \} \quad\text{and}\quad w(y):=v \bigg (\frac{y}{d^{1/2s}} \bigg ),\quad\text{where } y \in \Omega_{d}. \end{align*} $$

Now,

$$ \begin{align*} &d\int_{\Omega}\int_{\Omega} \frac{\vert v(x)-v(y)\vert^{2}}{\vert x-y\vert^{n+2s}}\,dx\,dy + \int_{\Omega}{v}^{2}\,dx\\&\quad= \frac{1}{d^{{n}/{2s}}} \bigg [ \int_{\Omega_{d}}\int_{\Omega_{d}} \frac{\vert v (\tfrac{x'}{d^{{1}/{2s}}} )-v(\tfrac{y'}{d^{{1}/{2s}}} )\vert^{2}}{\vert x'-y'\vert^{n+2s}}\,dx'\,dy' + \int_{\Omega_{d}}{v\bigg (\frac{x'}{d^{{1}/{2s}}} \bigg )}^{2}\,dx' \bigg ] \\&\quad= \frac{1}{d^{{n}/{2s}}} \bigg [ \int_{\Omega_{d}}\int_{\Omega_{d}} \frac{\vert w(x')-w(y')\vert^{2}}{\vert x'-y'\vert^{n+2s}}\,dx'\,dy' + \int_{\Omega_{d}}{w(x')}^{2}\,dx' \bigg ] \\&\quad\geq \frac{A}{d^{{n}/{2s}}} \bigg(\int_{\Omega_{d}}{\vert w\vert^{2_{s}^{*}}} \,dx' \bigg)^{{2}/{2_{s}^{*}}} \\&\quad= Ad^{({2}/{2_{s}^{*}}-1 ){n}/{2s}} \bigg(\int_{\Omega}{\vert v\vert^{2_{s}^{*}}} \,dx \bigg)^{{2}/{2_{s}^{*}}}. \end{align*} $$

Therefore, we observe that A is uniform for $d \in (0, d_{0}).$

It is easy to see that $\Omega \times \Omega \subset T(\Omega ).$ Then, by virtue of (3-10) and (3-11),

(3-12) $$ \begin{align} \bigg(\int_{\Omega}{\vert u_{d}\vert^{t2_{s}^{*}}} \bigg)^{{2}/{2_{s}^{*}}} \leq \frac{tA}{d}\int_{\Omega}u_{d}^{p+2t-1}\,dx. \end{align} $$

Now, we define two sequences $\{L_{j} \}$ and $\{M_{j} \}$ by the following recurrence relations:

(3-13) $$ \begin{align} p-1+2L_{0}= & \, 2_{s}^{*}, \nonumber \\ p-1+2L_{j+1}= & \, 2_{s}^{*}L_{j}, \quad j=0,1,2,\ldots \end{align} $$
(3-14) $$ \begin{align} M_{0}=& \, (AC_{0})^{{2_{s}^{*}}/{2}}, \nonumber \\ M_{j+1}=& \, (AL_{j}M_{j})^{{2_{s}^{*}}/{2}}, \quad j=0,1,2,\ldots \end{align} $$

We note that $L_{j}$ is explicitly given by

(3-15) $$ \begin{align} L_{j}=\frac{1}{(2_{s}^{*}-2)}\bigg( \bigg(\frac{2_{s}^{*}}{2}\bigg)^{j+1}(2_{s}^{*}-p-1)+p-1 \bigg). \end{align} $$

Since $1<p<2_{s}^{*}-1$ , it follows that $L_{j}\geq 1$ for all $j \geq 0$ and $L_{j} \rightarrow \infty $ as $j \rightarrow \infty .$ We show that

(3-16) $$ \begin{align} \int_{\Omega}u_{d}^{p-1+2L_{j}}\,dx \leq & \, M_{j}d^{{n}/{2s}} \quad\text{for all } j\geq 0, \end{align} $$

and

(3-17) $$ \begin{align} M_{j}\leq e^{mL_{j-1}} \end{align} $$

for some constant $m>0.$ Then,

$$ \begin{align*} \sup_{\Omega}u_{d}(x)\leq C_{1},\end{align*} $$

where $C_{1}>0$ depends only on $C_{0}$ and $\Omega .$ In fact, (3-15) and (3-16) give

$$ \begin{align*} \Vert u\Vert_{L^{2_{s}^{*}L_{j-1}}(\Omega)} &\leq ( e^{mL_{j-1}}d^{{n}/{2s}} )^{{1}/{(2_{s}^{*}L_{j-1})}} \nonumber \\ &= e^{{m}/{2_{s}^{*}} d^{{(n-2s)}/{4L_{j-1}}}} \end{align*} $$

and hence letting $j \rightarrow \infty ,$

$$ \begin{align*}\Vert u\Vert_{L^{\infty}(\Omega)} \leq e^{{m}/{2_{s}^{*}}}.\end{align*} $$

First, we verify (3-16). By virtue of (1-6) and (3-11),

$$ \begin{align*} \bigg(\int_{\Omega}{\vert u_{d}\vert^{2_{s}^{*}}} \bigg)^{{2}/{2_{s}^{*}}} &\leq \frac{A}{d}\bigg( \frac{c_{n,s}d}{2}\int_{T(\Omega)} \frac{\vert u_{d}(x)-u_{d}(y)\vert^{2}}{\vert x-y\vert^{n+2s}}\,dx\,dy + \int_{\Omega}\vert u_{d}\vert^{2}\,dx \bigg) \nonumber \\ &\leq \frac{A}{d}C_{0}d^{{n}/{2s}} \nonumber \\ &= AC_{0}d^{{n}/{s2_{s}^{*}}}. \end{align*} $$

Hence, (3-16) holds for $j=0.$ Suppose that we have proved (3-16) for $j \geq 0.$ Then, by (3-12),

$$ \begin{align*} \int_{\Omega}{\vert u_{d}\vert^{p-1+2L_{j+1}}}\,dx &\leq \bigg (\frac{L_{j}A}{d}\int_{\Omega}u_{d}^{p+2L_{j}-1}\,dx \bigg )^{{2_{s}^{*}}/{2}} \nonumber \\ &\leq ( AL_{j}d^{-1}M_{j}d^{{n}/{2s}} )^{{2_{s}^{*}}/{2}} \nonumber \\ &= (AL_{j}M_{j} )^{{2_{s}^{*}}/{2}}d^{{n}/{2s}}. \end{align*} $$

This implies that (3-16) is also true for $j+1.$ Therefore, it remains to show (3-17). Put

(3-18) $$ \begin{align} \lambda_{j}= & \, \frac{2_{s}^{*}}{2} \cdot \log(AL_{j}) \quad\text{and}\quad \eta_{j}= \log(M_{j}). \end{align} $$

Hence,

$$ \begin{align*} \eta_{j+1}=& \, \frac{2_{s}^{*}}{2}\cdot \eta_{j} +\lambda_{j}. \end{align*} $$

The explicit value of $L_{j}$ is given by

(3-19) $$ \begin{align} L_{j}= (2_{s}^{*}-2)^{-1} ( (2^{-1}2_{s}^{*})^{j+1}(2_{s}^{*}-p-1)+p-1 ). \end{align} $$

Now,

$$ \begin{align*} \lambda_{j}=& \, \frac{2_{s}^{*}}{2}\log\bigg[ \frac{A}{(2_{s}^{*}-2)}((2^{-1}2_{s}^{*})^{j+1}(2_{s}^{*}-p-1)+p-1 ) \bigg ]\\ =& \, \frac{2_{s}^{*}}{2} \bigg [ \log(A(2_{s}^{*}-2))+ \log ((2^{-1}2_{s}^{*})^{j+1}(2_{s}^{*}-p-1)+p-1 ) \bigg ].\nonumber \end{align*} $$

Therefore, we can find some $C^{*}$ such that

$$ \begin{align*} \lambda_{j} \leq C^{*}(j+1). \end{align*} $$

We now define a sequence $ \{\gamma _{j} \}$ by

(3-20) $$ \begin{align} \gamma_{0}= \eta_{0} \quad\text{and}\quad \gamma_{j+1}= \frac{2_{s}^{*}}{2}\gamma_{j} + C^{*}(j+1) \end{align} $$

for $j \geq 1.$ Clearly, $\eta _{j} \leq \gamma _{j}$ for all $j \geq 0.$ Moreover, since

$$ \begin{align*} \gamma_{j}= \bigg (\frac{2_{s}^{*}}{2} \bigg )^{j}( \eta_{0}+2C^{*}2_{s}^{*}(2_{s}^{*}-2)^{-2} )-2C^{*}(2_{s}^{*}-2)^{-1} (j+ 2_{s}^{*}(2_{s}^{*}-2)), \end{align*} $$

in view of (3-19), there exists $m>0$ such that $\gamma _{j} \leq mL_{j-1}.$ Hence, $\log (M_{j}) \leq m L_{j-1}$ and we obtain (3-17). Observe that m depends only on $\eta _{0}$ , $2_{s}^{*}$ and $C^{*},$ whereas $C^{*}$ depends only on $2_{s}^{*}$ , p and $A.$ This completes the proof.

Remark 3.5. It is known that if $u \in \mathcal {L}_{s}(\mathbb {R}^{n})\cap C^{2s+\epsilon }(\Omega ), $ when $0<s<\tfrac 12, 2s+\epsilon <1$ or $u \in \mathcal {L}_{s}(\mathbb {R}^{n})\cap C^{1,2s+\epsilon -1}(\Omega ), $ when $\tfrac 12\leq s<1, 2s+\epsilon -1<1$ , one can compute $(-\Delta )^{s}u(x)$ pointwise for all x in $\Omega .$ In fact, one can write

$$ \begin{align*} (-\Delta)^{s}u(x)=c_{n,s}\ \mathrm{PV} \int_{\mathbb{R}^{n}} \frac{u(x)-u(y)}{\vert x-y\vert^{n+2s}}\,dy. \end{align*} $$

Definition 3.6. We call $u: \mathbb {R}^{n} \longrightarrow \mathbb {R}$ a classical solution of (1-1) if it satisfies the following:

  1. (1) $u \in \mathcal {L}_{s}(\mathbb {R}^{n})\cap C^{2s+\epsilon }(\Omega ), $ when $0<s<\tfrac 12, 2s+\epsilon <1$ or $u \in \mathcal {L}_{s}(\mathbb {R}^{n})\cap C^{1,2s+\epsilon -1}(\Omega ), $ when $\tfrac 12\leq s<1, 2s+\epsilon -1<1;$

  2. (2) $\mathcal {N}_{s}u(x)=0, \,\,\, x \in \mathbb {R}^{n}\setminus \Omega ;$

  3. (3) $d(-\Delta )^{s}u(x)+u(x)= \vert u(x)\vert ^{p-1}u(x)$ pointwise for all $x \in \Omega .$

We make similar remarks as in [Reference Biagi, Dipierro, Valdinoci and Vecchi6], which offers a relation between the weak and classical solutions of (1-1).

Remark 3.7. Let $u_{d}$ be the least energy solution of (1-1) in $H^{s}_{\Omega }.$ Then, by Lemma 2.3, Theorem 1.2 and Lemma 3.4:

  1. (1) for $0<s<\tfrac 12$ , $u_{d} \in \mathcal {L}_{s}(\mathbb {R}^n)\cap C^{2}(\Omega )$ if $p>3-2s$ and $u_{d} \in \mathcal {L}_{s}(\mathbb {R}^n) \cap C^{1, p-2+2s}(\Omega )$ if $2<p\leq 3-2s$ ;

  2. (2) for $\tfrac 12 \leq s < 1$ , $u_d \in \mathcal {L}_{s}(\mathbb {R}^n) \cap C^{2}(\Omega ).$

Now, using the nonlocal integration by parts formulae given in [Reference Dipierro, Ros-Oton and Valdinoci14], one can easily check that

$$ \begin{align*} d(-\Delta)^{s}u_{d}(x) + u_{d}(x)=\vert u_{d}(x)\vert^{p-1}u_{d}(x) \end{align*} $$

holds pointwise in $\Omega .$ This implies that $u_{d}$ is a classical solution of (1-1). Conversely, if $u_{d}$ is a classical solution of (1-1) satisfying $u_{d} \in H^{s}_{\Omega },$ then $u_{d}$ is a weak solution of (1-1).

The following lemma shows that the maximum of the least energy solution is always greater than unity.

Lemma 3.8. Let $u_d$ be the least energy solution of (1-1). Let

$$ \begin{align*} M_{d}=\sup_{x\in \overline{\Omega}} u_{d}(x). \end{align*} $$

Then, $M_{d}>1.$

Proof. Since $u_{d}$ is a weak solution of (1-1),

$$ \begin{align*} &d\frac{c_{n,s}}{2}\int_{T(\Omega)}\frac{(u_{d}(x)-u_{d}(y))(w(x)-w(y))}{\vert x-y\vert^{n+2s}}\,dx\,dy + \int_{\Omega}u_{d}w \,dx =\int_{\Omega} u_{d}^{p}w \,dx \end{align*} $$

holds for all $w \in H_{\Omega}^{s}$ . Taking $w=1$ in the above equation,

$$ \begin{align*} \int_{\Omega}u_{d}(x)\,dx=& \,\int_{\Omega}u_{d}^{p}(x)\,dx. \end{align*} $$

This implies that

$$ \begin{align*} \int_{\Omega}u_{d}(x)(1-u_{d}^{p-1}(x))\,dx=& \,0. \end{align*} $$

Now, if $u_{d}(x)\leq 1$ for all $x \in \overline {\Omega },$ then

$$ \begin{align*}1-u_{d}(x)\geq 0 \quad\text{for all } x \in {\overline{\Omega}} .\end{align*} $$

Thus, from the above equation, we get that $u_{d}(x)= 1~a.e.$ in $\overline {\Omega }.$ Now, by Lemma 3.4, we can assume that $u_{d}$ is continuous and hence $u_{d}\equiv 1$ in $\overline {\Omega },$ which is a contradiction to our assumption that $u_{d}$ is a nonconstant solution. Therefore, there exists $x_{0}$ in $\overline {\Omega }$ such that $u_{d}(x_{0})>1.$ Thus, $M_{d}>1.$

4. $L^{r}$ -estimates on $u_{d}$

Here, we derive an $L^{r}$ -estimate for $u_{d}.$ The following results are generalisations of [Reference Lin, Ni and Takagi31, Proposition 2.2 and Lemma 2.3] to the nonlocal case.

Proposition 4.1. For $d_{0}>0$ fixed, there is a constant $K_{0}$ such that

(4-1) $$ \begin{align} d\frac{c_{n,s}}{2}\int_{T(\Omega)}\frac{(u_{d}(x)-u_{d}(y))^{2}}{\vert x-y\vert^{n+2s}}\,dx\,dy + \int_{\Omega}u_{d}^{2} \,dx \geq K_{0}d^{{n}/{2s}}, \end{align} $$

where $u_{d}$ is the least energy solution of (1-1) with $0<d<d_{0}.$

Proof. In contrast, suppose that there is a sequence $\{d_{k}\}$ contained in the interval $(0,d_{0})$ and a sequence of positive solutions $\{u_{k}\}$ to (1-1) with $d=d_{k}$ such that

$$ \begin{align*} \zeta_{k}:= \frac{1}{d^{{n}/{2s}}}\bigg(d \frac{c_{n,s}}{2} \int_{T(\Omega)}\frac{(u_{k}(x)-u_{k}(y))^{2}}{\vert x-y\vert^{n+2s}}\,dx\,dy + \int_{\Omega}u_{k}^{2} \,dx \bigg) \rightarrow 0 \quad\text{as } k\rightarrow \infty. \end{align*} $$

We are going to follow the same arguments as used in the proof of Lemma 1.2 to prove this proposition. Once again, define the sequences $\{L_{k}\}$ and $\{M_{j}\}$ as defined earlier in (3-13) and (3-14), respectively. Instead of $C_{0},$ we write $\zeta _{k}$ in the definition of $\{M_{j}\}$ :

$$ \begin{align*} p-1+2L_{0}= & \, 2_{s}^{*}, \nonumber \\ p-1+2L_{j+1}= & \, 2_{s}^{*}L_{j}, \quad j=0,1,2,\ldots \end{align*} $$

and

$$ \begin{align*} M_{0}=& \, (A\zeta_{k})^{{2_{s}^{*}}/{2}}, \nonumber \\ M_{j+1}=& \, (AL_{j}M_{j})^{{2_{s}^{*}}/{2}}, \quad j=0,1,2,\ldots. \end{align*} $$

Further, define the sequences $\{\lambda _{j}\}$ , $\{\eta _{j}\}$ and $\{\gamma _{j}\}$ as defined earlier in (3-18) and (3-20). From (3-16),

(4-2) $$ \begin{align} \bigg(\int_{\Omega}u_{k}^{2_{s}^{*}L_{j-1}}\,dx\bigg)^{(2_{s}^{*}L_{j-1})} \leq & \, (M_{j}d_{k}^{n/2s} )^{1/(2_{s}^{*}L_{j-1})}. \end{align} $$

Since

$$ \begin{align*}\log(M_{j})=\eta_{j} \leq \gamma_{j},\end{align*} $$

we have

$$ \begin{align*} \frac{\log(M_{j})}{2_{s}^{*}L_{j-1}} \leq \frac{\eta_{j}}{2_{s}^{*}L_{j-1}}. \end{align*} $$

Now,

$$ \begin{align*} \lim_{j \rightarrow \infty} \frac{\eta_{j}}{2_{s}^{*}L_{j-1}}&= \lim_{j \rightarrow \infty}\frac{\big(\tfrac{2_{s}^{*}}{2}\big)^{j}[ \eta_{0}+2C^{*}2_{s}^{*}(2_{s}^{*}-2)^{-2} ]-2C^{*}(2_{s}^{*}-2)^{-1} [j+ 2_{s}^{*}(2_{s}^{*}-2)]}{\tfrac{2_{s}^{*}}{(2_{s}^{*}-2)}\Big [ \big(\tfrac{2_{s}^{*}}{2}\big)^{j}(2_{s}^{*}-p-1)+p-1 \Big ]}\\[3pt] &= \frac{(2_{s}^{*}-2)(\eta_{0}+2C^{*}2_{s}^{*}(2_{s}^{*}-2)^{-2})}{2_{s}^{*}(2_{s}^{*}-p-1)}. \end{align*} $$

Letting $j \rightarrow \infty $ in (4-2),

(4-3) $$ \begin{align} \Vert u_{k}\Vert_{L^{\infty}(\Omega)} \leq e^{a_{1}(\eta_{0}+a_{2})}, \end{align} $$

with $a_{1}$ and $a_{2}$ depending only on $2_{s}^{*},~p$ and $C^{*}.$ Since

$$ \begin{align*} \eta_{0}= \log (M_{0})= \frac{2_{s}^{*}}{2}\log(A\zeta_{k}), \end{align*} $$

as $k \rightarrow \infty ,~\eta _{0}\rightarrow -\infty .$ Thus, in view of (4-3),

$$ \begin{align*} \Vert u_{k}\Vert_{L^{\infty}(\Omega)} \rightarrow 0, \end{align*} $$

which leads to a contradiction to Lemma 3.8.

Proof of Theorem 1.3

First, we show the second part of (1-7).

Case I. $r \geq 2_{s}^{*}={2n}/({n-2s}).$ Let $\{L_{j} \}$ be the sequence defined in (3-13). If $r \in \{2_{s}^{*}L_{j} \}$ , then the second inequality of (1-7) follows from (3-16). So assume that $2_{s}^{*}L_{j}<r< 2_{s}^{*}L_{j+1}$ for some $j \geq 0.$ We have

$$ \begin{align*}r=t2_{s}^{*}L_{j}+(1-t)2_{s}^{*}L_{j+1} \text{ for some } t \in (0,1).\end{align*} $$

Using the Hölder inequality and (3-16),

$$ \begin{align*} \int_{\Omega}u_{d}^{r}\,dx = & \, \int_{\Omega}u_{d}^{t2_{s}^{*}L_{j}+(1-t)2_{s}^{*}L_{j+1}}\,dx, \\ \leq & \, \bigg( \int_{\Omega}u_{d}^{2_{s}^{*}L_{j}}\,dx \bigg)^{t}\bigg( \int_{\Omega}u_{d}^{2_{s}^{*}L_{j+1}}\,dx \bigg)^{1-t} \\ \leq & \, (M_{j-1}d^{n/2s} )^{t}(M_{j}d^{n/2s})^{1-t}\\ = & \, M_{j-1}^{t}M_{j}^{1-t}d^{{n}/{2s}}. \end{align*} $$

Case II. $2 \leq r \leq 2_{s}^{*}$ . We write

$$ \begin{align*}r=2t+(1-t)2_{s}^{*}, \end{align*} $$

for some $t \in [0,1].$ Then, using the Hölder inequality, from (1-6) and (3-16) with $j=0$ ,

$$ \begin{align*} \int_{\Omega}u_{d}^{r}\,dx \leq & \, \bigg( \int_{\Omega}u_{d}^{2}\,dx \bigg)^{t} \bigg( \int_{\Omega}u_{d}^{2_{s}^{*}}\,dx \bigg)^{1-t}\\ \leq & \, C_{0}^{t}M_{0}^{(1-t)}d^{{n}/{2s}}, \end{align*} $$

where the constant $C_{0}$ is independent of $d.$

Case III. $1 \leq r < p+1.$ Integrating both sides of (1-1) and using the condition $\mathcal {N}_{s}u(x)=0$ for $x\in \mathcal {C}\Omega ,$

(4-4) $$ \begin{align} \int_{\Omega}u_{d}\,dx= \int_{\Omega}u_{d}^{p}\,dx. \end{align} $$

It is easy to see that

$$ \begin{align*} p=t+(1-t)(p+1) \quad\text{with } t=\frac{1}{p} \in (0,1). \end{align*} $$

Notice that $p+1 \in (2, 2_{s}^{*}).$ Therefore, using the Hölder inequality and (4-4),

$$ \begin{align*} \int_{\Omega}u_{d}^{p}\,dx \leq & \, \bigg( \int_{\Omega}u_{d}\,dx \bigg)^{t}\bigg( \int_{\Omega}u_{d}^{p+1}\,dx \bigg)^{(1-t)}, \\ \int_{\Omega}u_{d}^{p}\,dx \leq & \, \int_{\Omega}u_{d}^{p+1}\,dx \leq C_{0}d^{{n}/{2s}} \quad (\text{by}\ ({1\text{-}6})), \end{align*} $$

where the constant $C_{0}$ depends only upon $p+1.$

Also, in view of (4-4) and (1-6), we observe that the second inequality of (1-7) holds for $r=1.$ Now, repeating the interpolation between $1$ and $p+1$ , we see that the second inequality of (1-7) holds for all r $\geq 1.$

Case IV. Let $0<r \leq 1.$ Taking $F=u_{d}^{r},\, G=1, \, p=\frac {1}{r}, \, q=\frac {1}{1-r}$ and using the Hölder inequality,

$$ \begin{align*} \int_{\Omega}u_{d}^{r}\,dx \leq \Vert F\Vert_{p}\Vert G\Vert_{q}=\vert\Omega\vert^{1-r} \bigg(\int_{\Omega}u_{d}\,dx \bigg)^{r} \leq \vert\Omega\vert^{1-r} B(1)^{r}d^{{nr}/{2s}}. \end{align*} $$

This proves the second inequality of (1-8).

Now, let us prove the first inequality of (1-7) and (1-8). In view of (3-5) and (4-1),

$$ \begin{align*} \int_{\Omega}u_{d}^{p+1} \geq K_{0}d^{{n}/{2s}}. \end{align*} $$

Since

$$ \begin{align*}\displaystyle \sup_{\Omega}u_{d}(x) \leq C_{1}\quad \text{for some constant } C_{1}>0,\end{align*} $$

we have

$$ \begin{align*} K_{0}d^{{n}/{2s}}\leq \int_{\Omega}u_{d}^{p+1} &= \, \int_{\Omega}(u_{d}^{p+1-r})(u_{d}^{r})\,dx \\ &\leq C_{1}^{p+1-r}\int_{\Omega}u_{d}^{r}\,dx. \end{align*} $$

This implies that

$$ \begin{align*}\int_{\Omega}u_{d}^{r}\,dx \geq K_{0}C_{1}^{r-p-1}d^{{n}/{2s}}, ~r<p+1.\end{align*} $$

For $r>p+1$ , we write $p+1=1+(1-t)r.$ Therefore,

$$ \begin{align*} K_{0}d^{{n}/{2s}}\leq & \, \int_{\Omega}u_{d}^{p+1}\,dx \\ =& \, \int_{\Omega}u_{d}^{1+(1-t)r}\,dx \\ \leq & \, (u_{d}\,dx )^{t}(u_{d}^{r}\,dx )^{1-t} \\ \leq & \, ( B(1)d^{{n}/{2s}} )^{t} ( u_{d}^{r}\,dx )^{1-t}. \end{align*} $$

This yields that

$$ \begin{align*}\int_{\Omega}u_{d}^{r}\,dx \geq (K_{0}B(1)^{-t})^{{1}/({1-t})}d^{{n}/{2s}}.\\[-41pt] \end{align*} $$

5. Proof of Theorem 1.4

In this section, we prove Theorem 1.4. Its proof is intricate and requires some scaling and compactness arguments. We prove the statements of the theorem one by one. Let $z_{d} \in \overline {\Omega } $ be a point of maximum of $u_{d}.$ We approximate $u_{d}$ around $z_{d}$ by a scaled positive radial solution of (1-5). It gives us an upper bound on $c_{d},$ which is closely related to the location of point $z_{d}.$

Step I. We prove that there exists a positive constant $K_{*}$ such that

(5-1) $$ \begin{align} \rho (z_{d}, \partial \Omega) \leq K_{*}d^{{1}/{2s}} .\end{align} $$

If the inequality in (5-1) is not true, then there is a decreasing sequence $d_{j}\downarrow 0$ such that

(5-2) $$ \begin{align} \rho_{j}:=\frac{\rho(z_{j}, \partial \Omega)}{d_{j}^{{1}/{2s}}} \rightarrow +\infty \quad\text{as } j \rightarrow \infty, \end{align} $$

where $z_{j}:=z_{d_{j}}$ is a point of maximum of $u_{d_{j}}$ on $\overline {\Omega }.$ Define

$$ \begin{align*}\phi_{j}(y):=u_{d_{j}}(yd_{j}^{{1}/{2s}}+z_{j}) \quad \text{for } y \in \mathbb{R}^{n}.\end{align*} $$

Since $u_{d}$ is a classical solution of (1-1),

(5-3) $$ \begin{align} (-\Delta)^{s}\phi_{j}+\phi_{j}=\phi_{j}^{p} \quad \text{in } B_{\rho_{j}}, \end{align} $$

and:

  1. (1) $ \phi _{j} \in C^{0,2s+\epsilon }(B_{\rho _{j}}),$ when $0<s<\tfrac 12$ , $ 2s+\epsilon <1; $

  2. (2) $ \phi _{j} \in C^{1,2s+\epsilon -1}(B_{\rho _{j}}),$ when $\tfrac 12 \leq s <1$ , $2s+\epsilon -1<1.$

First, we claim that the sequence $\{\phi _{j}\}$ contains a convergent subsequence. Let $\{R_{k}\}$ be a monotone increasing sequence of positive numbers with $R_{k} \rightarrow +\infty $ as $k \rightarrow \infty .$ Therefore, we have for each $k,$ there is a number $j_{k}$ such that $4R_{k}< \rho _{j}$ whenever $j \geq j_{k}.$ Since $u_{d} \in L^{\infty }(\mathbb {R}^n) \cap \mathcal {L}_{s}(\mathbb {R}^n),$ we have $ \phi _{{j}} \in L^{\infty }(\mathbb {R}^n) \cap \mathcal {L}_{s}(\mathbb {R}^n)$ for each $j \geq 1.$ Now, we can use [Reference Fall19, Theorem 1.4] to get the following estimates.

For $0<s<\tfrac 12$ , $ 2s+\epsilon <1$ :

  1. (i) let $4s+\epsilon <1,$ then

    $$ \begin{align*} \Vert\phi_{{j}}\Vert_{C^{0,4s+\epsilon} (B_{2R_{k}})} \leq C (\Vert\phi_j\Vert_{L^{\infty} (\mathbb{R}^{n})} + \Vert\phi_{j}^{p}-\phi_j\Vert_{C^{0,2s+\epsilon}(B_{4R_{k}})} ); \end{align*} $$
  2. (ii) let $1<4s+\epsilon <2,$ then

    $$ \begin{align*} \Vert\phi_{{j}}\Vert_{C^{1,4s+\epsilon-1} (B_{2R_{k}})} \leq C (\Vert\phi_j\Vert_{L^{\infty} (\mathbb{R}^{n})} + \Vert\phi_{j}^{p}-\phi_j\Vert_{C^{0,2s+\epsilon}(B_{4R_{k}})} ); \end{align*} $$

and for $\tfrac 12 \leq s <1$ , $2s+\epsilon -1<1$ :

  1. (iii) let $4s+\epsilon -1<1,$ then

    $$ \begin{align*} \Vert\phi_{{j}}\Vert_{C^{1,4s+\epsilon-1} (B_{2R_{k}})} \leq C (\Vert\phi_j\Vert_{L^{\infty} (\mathbb{R}^{n})} + \Vert\phi_{j}^{p}-\phi_j\Vert_{C^{1,2s+\epsilon-1}(B_{4R_{k}})} ); \end{align*} $$
  2. (iv) let $1<4s+\epsilon -1<2,$ then

    $$ \begin{align*} \Vert\phi_{{j}}\Vert_{C^{2,4s+\epsilon-1} (B_{2R_{k}})} \leq C (\Vert\phi_j\Vert_{L^{\infty} (\mathbb{R}^{n})} + \Vert\phi_{j}^{p}-\phi_j\Vert_{C^{1,2s+\epsilon-1}(B_{4R_{k}})} ), \end{align*} $$

where the constant $C>0$ is independent of $j.$

Let us recall the inequality (1-6) here:

$$ \begin{align*} d \frac{c_{n,s}}{2} \int_{T(\Omega)} \frac{\vert u_{d}(x)-u_{d}(y)\vert^{2}}{\vert x-y\vert^{n+2s}}\,dx\,dy + \int_{\Omega}u^{2}\,dx=\int_{\Omega} u_{d}^{p+1} \leq C_{0}d^{{n}/{2s}}, \end{align*} $$

where $C_{0}$ is independent of $d.$ This yields

$$ \begin{align*} \int_{B_{\rho_{j}}} \phi_{j}^{p+1} \leq C_{0}, \end{align*} $$

and

(5-4) $$ \begin{align} \Vert\phi_{j}\Vert_{H^{s}(B_{\rho_{j}})} \leq C_{0} \quad\text{for all } j\geq 1. \end{align} $$

Also, by Theorem 1.3,

$$ \begin{align*} \int_{\Omega} u_{d}^{r} \leq B(r)d^{{n}/{2s}} \quad \text{for all } r \geq 1, \end{align*} $$

which implies that

(5-5) $$ \begin{align} \int_{B_{\rho_{j}}} \phi_{j}^r \leq B(r)\quad\text{for all } j\geq 1 \text{ and } r \geq 1. \end{align} $$

By Lemma 3.4 and Theorem 1.2,

(5-6) $$ \begin{align} \Vert u_{d}\Vert_{L^{\infty}(\mathbb{R}^{n})} \leq C_{1}, \end{align} $$

where the constant $C_{1}$ is independent of the diffusion constant $d.$ So, (5-5), (5-6) and [Reference Fall19, Theorem 1.3] imply that

$$ \begin{align*} \Vert\phi_{j}\Vert_{X_{s}(\overline{B}_{R_{k}})} < C_2 \quad \text{for all } j \geq j_{k}, \end{align*} $$

where the constant $C_2>0$ is independent of j and the space $X_{s}(\overline {B}_{R_{k}})$ is identified with one of the spaces $C^{0,4s+\epsilon }(\overline {B}_{R_{k}})$ , $C^{1,4s+\epsilon -1}(\overline {B}_{R_{k}})$ or $C^{2,4s+\epsilon -1}(\overline {B}_{R_{k}})$ with the same assumptions on s and $\epsilon $ as above. Therefore, $\{\phi _{j}\}$ is a relatively compact set in $X_{s}(\overline {B}_{R_{k}}),$ and hence by the standard diagonal process, we can extract a convergent subsequence of $\{\phi _{j}\},$ which we continue to denote by $\{\phi _{j}\}$ itself such that

$$ \begin{align*} \phi_{j} \rightarrow v \quad \text{in } C^{0, 2s+\epsilon}_{loc}(\mathbb{R}^{n}) \quad\text{when } 0<s<\tfrac{1}{2}, 2s+\epsilon<1 \end{align*} $$

or

$$ \begin{align*} \phi_{j} \rightarrow v \quad \text{in } C^{1, 2s+\epsilon-1}_{loc}(\mathbb{R}^{n}) \quad\text{when } \tfrac{1}{2}<s<1, 2s+\epsilon-1<1 \end{align*} $$

for some $v.$ The limit $v \in C^{0,2s+\epsilon }(\mathbb {R}^{n}) \cap H^{s}(\mathbb {R}^{n})$ when $0<s<\tfrac 12, 2s+\epsilon <1$ or $v \in C^{1,2s+\epsilon -1}(\mathbb {R}^{n}) \cap H^{s}(\mathbb {R}^{n})$ when $\tfrac 12<s<1, 2s+\epsilon -1<1$ follows from (5-4). Consequently,

$$ \begin{align*} \lim_{\vert x\vert\rightarrow \infty}v(x)=0. \end{align*} $$

Using [Reference Du, Jin, Xiong and Yang17, Theorem 1.1], we have $(-\Delta )^{s}\phi _{j}(x) $ converges to $ (-\Delta )^{s}v(x)$ point-wise in $\mathbb {R}^{n}.$ Consequently, we see that the limit v satisfies the equation

$$ \begin{align*} (-\Delta)^{s}v+v=v^{p} \quad \text{in } \mathbb{R}^{n}. \end{align*} $$

Clearly, $v \geq 0$ because each $\phi _{j} \geq 0.$ Since by Lemma 3.8 we have $\phi _{j}(0)=u_{d_{j}}(z_{j})>1$ for each $j \geq 1,$ one can see that $v \not \equiv 0.$

Using Theorem 2.9, one can see that v is radially symmetric and decreasing about some point in $\mathbb {R}^{n}.$ Since

$$ \begin{align*} \nabla v(0)= \lim_{j \rightarrow \infty} \nabla \phi_{j}(0)=0, \end{align*} $$

v is radially symmetric about the origin. Additionally, by Theorem 2.8, v has a power type of decay at infinity, that is,

$$ \begin{align*} v(r)\leq \frac{C_{2}}{r^{n+2s}}, \quad r \geq 1. \end{align*} $$

Now we derive a lower bound on the critical value $c_{d_{j}}.$ Let us define

(5-7) $$ \begin{align} \delta_{R}:= \frac{C_{2}}{R^{n+2s}}, \end{align} $$

where $R>0$ is an arbitrarily large real number. Then, there exists a positive integer $j_{R}$ such that if $j \geq j_{R}$ , then $\rho _{j}\geq 2R$ and

(5-8) $$ \begin{align} \Vert\phi_{j}-v\Vert_{C^{2}(\overline{B}_{2R})} \leq \delta_{R}. \end{align} $$

By Lemma 3.3,

$$ \begin{align*}c_{d_{j}}= M[u_{d_{j}}]=J_{d_{j}}(u_{d_{j}}).\end{align*} $$

Using this fact and (3-6),

$$ \begin{align*} c_{d_{j}}&= \bigg(\frac{1}{2}-\frac{1}{p+1}\bigg)\int_{\Omega}u_{d_{j}}^{p+1}\,dx \\ &\geq \bigg(\frac{1}{2}-\frac{1}{p+1}\bigg) \int_{\vert x-z_{j}\vert<d_{j}^{{1}/{2s}}R}u_{d_{j}}^{p+1}\,dx \nonumber \\ &= d_{j}^{{n}/{2s}} \bigg(\frac{1}{2}-\frac{1}{p+1}\bigg) \int_{\vert y\vert < R} \phi_{j}^{p+1}\,dy. \nonumber \end{align*} $$

Now,

(5-9) $$ \begin{align} c_{d_{j}}=& \, d_{j}^{{n}/{2s}} \bigg(\bigg(\frac{1}{2}-\frac{1}{p+1}\bigg)\int_{B_{R}} v^{p+1}\,dy+ F_{j} \bigg), \end{align} $$

where

$$ \begin{align*}F_{j}:= \bigg(\frac{1}{2}-\frac{1}{p+1}\bigg) \int_{B_{R}}\bigg( \phi_{{j}}^{p+1}- v^{p+1} \bigg)\,dy. \end{align*} $$

By Equation (5-8), we have for all $y \in B_{R},~ j \geq j_{R}$ ,

$$ \begin{align*} \vert \phi_{{j}}^{p+1}- v^{p+1}\vert \leq C \vert\phi_{{j}}-v\vert \leq \delta_{R}, \end{align*} $$

where $C>0$ is some constant. This implies that

$$ \begin{align*} \vert F_{j}\vert \leq \bigg(\frac{1}{2}-\frac{1}{p+1}\bigg)C \vert B_{R}\vert \delta_{R}=C_{3}R^{n}\delta_{R}, \end{align*} $$

where

$$ \begin{align*}C_{3}= \bigg(\frac{1}{2}-\frac{1}{p+1}\bigg)\frac{w_{n}}{n} C\end{align*} $$

and $w_{n}$ denotes the surface area of the unit sphere in $\mathbb {R}^{n}.$ Consequently, (5-9) becomes

(5-10) $$ \begin{align} c_{d_{j}}\geq d_{j}^{{n}/{2s}} \bigg[\bigg(\frac{1}{2}-\frac{1}{p+1}\bigg)\int_{B_{R}} v^{p+1}\,dy-C_{3}R^{n}\delta_{R} \bigg]. \end{align} $$

Now, it is easy to see that

$$ \begin{align*} \bigg(\frac{1}{2}-\frac{1}{p+1}\bigg)\int_{B_{R}} v^{p+1}\,dy= F(v)-\bigg(\frac{1}{2}-\frac{1}{p+1}\bigg)\int_{\vert y\vert>R} v^{p+1}\,dy, \end{align*} $$

where $F(v)$ is defined earlier in (2-2). Simplifying the second term on right-hand side,

$$ \begin{align*} \bigg(\frac{1}{2}-\frac{1}{p+1}\bigg)\int_{\vert y\vert>R} v^{p+1}\,dy&= \, \bigg(\frac{1}{2}-\frac{1}{p+1}\bigg) \int_{R}^{\infty} \frac{r^{n-1}w_{n}}{r^{(n+2s)(p+1)}}\,dr \\ &= \, \bigg(\frac{1}{2}-\frac{1}{p+1}\bigg) \frac{w_{n}}{(n+2s)p+2s}\frac{1}{R^{(n+2s)p+2s}}=\frac{C_{4}}{R^{(n+2s)p+2s}}. \end{align*} $$

Therefore, one can write

(5-11) $$ \begin{align} \bigg(\frac{1}{2}-\frac{1}{p+1}\bigg)\int_{B_{R}} v^{p+1}\,dy = F(v)-\frac{C_{4}}{R^{(n+2s)p+2s}}. \end{align} $$

On combining (5-7), (5-10) and (5-11), we get for $j \geq j_{R},$

(5-12) $$ \begin{align} c_{d_{j}} &\geq d_{j}^{{n}/{2s}}\bigg( F(v)- \frac{C_{4}}{R^{(n+2s)p+2s}}-\frac{C_{2}C_{3}}{R^{2s}} \bigg) \nonumber \\ &\geq d_{j}^{{n}/{2s}}\bigg( F(v)- \frac{C_{5}}{R^{2s}} \bigg) , \end{align} $$

where $C_{5}$ is independent of j and $R.$

Now, we derive an upper bound on the critical value $c_{d_{j}}.$ Without loss of generality, we may assume that the domain $\Omega $ is a subset of $\mathbb {R}^{n}_{+}$ and $0 \in \partial \Omega .$ Given Definition 2.13, let w be the ground state solution of (1-5). Define

$$ \begin{align*} \Omega_{d}&:=\bigg\{\frac{x}{d^{{1}/{2s}}} \mid x\in \Omega \bigg\},\\ w_{d}(x)&:=w\bigg( \frac{x}{d^{{1}/{2s}}}\bigg), \quad\text{for } x\in \mathbb{R}^{n}. \end{align*} $$

Since $w \geq 0$ , this implies that $w_{d} \geq 0$ . Define

$$ \begin{align*}g_{d}(t):=J_{d}(tw_{d}),\quad t \geq 0.\end{align*} $$

Then, by Lemma 3.3, there exists a unique $t_{0}=t_{0}(d)>0$ at which $g_{d}$ attains a maximum. It is easy to see that $t_{0}(d) \rightarrow 1$ as $d \downarrow 0.$ Hence,

$$ \begin{align*} M[w_{d}]&= J_{d}\bigg(t_{0}w_{d}\bigg) \\&= \frac{t_{0}^{2}}{2} \bigg[\frac{dc_{n,s}}{2}\int_{T(\Omega)}\frac{\vert w_{d}(x)-w_{d}(y)\vert^{2}}{\vert x-y\vert^{n+2s}}\,dx\,dy+ \int_{\Omega}w_{d}^{2}\,dx\bigg]-\frac{t_{0}^{p+1}}{p+1}\int_{\Omega}w_{d}^{p+1}\,dx \\&= \frac{t_{0}^{2}}{2} \bigg[\frac{dc_{n,s}}{2}\int_{T(\Omega)}\frac{\bigg\vert w\bigg(\dfrac{x}{d^{{1}/{2s}}}\bigg)-w\bigg(\dfrac{y}{d^{{1}/{2s}}}\bigg)\bigg\vert^{2}}{\vert x-y\vert^{n+2s}}\,dx\,dy + \int_{\Omega}w^{2}\bigg(\frac{x}{d^{{1}/{2s}}}\bigg)\,dx\bigg]\\&\quad -\frac{t_{0}^{p+1}}{p+1}\int_{\Omega}w^{p+1}\bigg(\frac{x}{d^{{1}/{2s}}}\bigg)\,dx. \end{align*} $$

The change of variables

$$ \begin{align*} \frac{x}{d^{{1}/{2s}}}=a,\, \frac{y}{d^{{1}/{2s}}}=b, \end{align*} $$

gives us

$$ \begin{align*} M[w_{d}]&= d^{{n}/{2s}} \bigg(\frac{t_{0}^{2}}{2} \bigg[\frac{c_{n,s}}{2}\int_{T(\Omega_{d})}\frac{\vert w(a)-w(b)\vert^{2}}{\vert a-b\vert^{n+2s}}\,da\,db+ \int_{\Omega_{d}}w^{2}\,da\bigg]-\frac{t_{0}^{p+1}}{p+1}\int_{\Omega_{d}}w^{p+1}\,da \bigg) \\&= d^{{n}/{2s}} I_d \end{align*} $$

where $I_{d}$ is the expression

$$ \begin{align*} &\frac{t_{0}^{2}}{2} \bigg[\frac{c_{n,s}}{2}\!\int_{\Omega_{d}}\! \int_{\Omega_{d}}\! \frac{\vert w(a)-w(b)\vert^{2}}{\vert a-b\vert^{n+2s}}\,da\,db+ 2c_{n,s}\int_{\mathcal{C}\Omega_{d}}\! \int_{\Omega_{d}}\! \frac{\vert w(a)-w(b)\vert^{2}}{\vert a-b\vert^{n+2s}}\,da\,db +\! \int_{\Omega_{d}}\!w^{2}\,da\bigg]\\&\quad -\frac{t_{0}^{p+1}}{p+1}\int_{\Omega_{d}}w^{p+1}\,da. \end{align*} $$

Since

$$ \begin{align*} t_{0}(d) \rightarrow 1 \quad\text{as }d\downarrow 0, \end{align*} $$

we get for $I_d$

$$ \begin{align*} &\frac{1}{2} \bigg[\frac{c_{n,s}}{2}\!\int_{\mathbb{R}^{n}_{+}} \!\int_{\mathbb{R}^{n}_{+}}\! \frac{\vert w(a)-w(b)\vert^{2}}{\vert a-b\vert^{n+2s}}\,da\,db+ 2c_{n,s}\!\int_{\mathcal{C} \mathbb{R}^{n}_{+}}\! \int_{\mathbb{R}^{n}_{+}}\! \frac{\vert w(a)-w(b)\vert^{2}}{\vert a-b\vert^{n+2s}}\,da\,db + \!\int_{\mathbb{R}^{n}_{+}}\! w^{2}\,da\bigg]\\&\quad -\frac{1}{p+1}\int_{\mathbb{R}^{n}_{+}}w^{p+1}\,da + o(1)\end{align*} $$

as $d \downarrow 0.$ Further, w being nonnegative and radially symmetric implies that

$$ \begin{align*}\int_{\mathbb{R}^{n}_{+}}w^{2}\,da=\frac{1}{2}\int_{\mathbb{R}^{n}}w^{2}\,da,\,\, \int_{\mathbb{R}^{n}_{+}}w^{p+1}\,da=\frac{1}{2}\int_{\mathbb{R}^{n}}w^{p+1}\,da,\end{align*} $$
$$ \begin{align*}\int_{\mathbb{R}^{n}_{+}} \int_{\mathbb{R}^{n}_{+}} \frac{\vert w(a)-w(b)\vert^{2}}{\vert a-b\vert^{n+2s}}\,da\,db = \frac{1}{4} \int_{\mathbb{R}^{n}} \int_{\mathbb{R}^{n}} \frac{\vert w(a)-w(b)\vert^{2}}{\vert a-b\vert^{n+2s}}\,da\,db,\end{align*} $$
$$ \begin{align*} \int_{\mathcal{C}\mathbb{R}^{n}_{+}} \int_{\mathbb{R}^{n}_{+}} \frac{\vert w(a)-w(b)\vert^{2}}{\vert a-b\vert^{n+2s}}\,da\,db = \frac{1}{4} \int_{\mathbb{R}^{n}} \int_{\mathbb{R}^{n}} \frac{\vert w(a)-w(b)\vert^{2}}{\vert a-b\vert^{n+2s}}\,da\,db.\end{align*} $$

Using these estimates,

$$ \begin{align*} I_{d} &< \frac{1}{2}\bigg( \frac{1}{2} \bigg[ \frac{c_{n,s}}{2}\int_{\mathbb{R}^{n}} \int_{\mathbb{R}^{n}} \frac{\vert w(a)-w(b)\vert^{2}}{\vert a-b\vert^{n+2s}}\,da\,db + \int_{\mathbb{R}^{n}}w^{2}\,da \bigg]- \frac{1}{p+1} \int_{\mathbb{R}^{n}}w^{p+1}\,da\bigg)+ o(1)\\& = \frac{1}{2}F(w)+o(1),\end{align*} $$

as $d \downarrow 0.$ Thus,

$$ \begin{align*} M[w_{d}]=d^{{n}/{2s}}I_{d}< \frac{d^{{n}/{2s}}}{2}F(w)+o(1), \end{align*} $$

as $d\downarrow 0.$ Using part (c) of Theorem 2.12, we have $0<F(w) \leq F(v)$ for any nonnegative nonzero classical solution v of (1-5) and by Lemma 3.3,

$$ \begin{align*}c_{d_{j}} \leq M[w_{d_{j}}]< \frac{d_{j}^{{n}/{2s}}}{2}F(v)\end{align*} $$

for $d_{j}$ sufficiently small. By letting R be sufficiently large in (5-12), we reach a contradiction. This proves (5-1).

Remark 5.1. In the classical case [Reference Ni and Takagi35], the authors have defined diffeomorphisms, which straighten a boundary portion near $Q \in \partial \Omega .$ Further, using scaling and translations of the least energy solutions $u_{d}$ of (1-3), the classical problem (1-3) gets transferred into a new elliptic equation. Due to the nonlocal nature of the fractional Laplacian and of the boundary condition in our problem, it seems almost impossible to introduce such scaling and translation arguments.

Step II. Now, we claim that $z_{d} \in \partial \Omega .$ Suppose that there is a decreasing sequence $d_{j} \downarrow 0$ such that $z_{d_{j}}:=z_{j} \in \Omega .$ We have from Lemma 1.4 that the sequence $\{z_{j}\}$ converges to some $z \in \partial \Omega .$ Without loss of generality, let us assume that $z=0.$ Define

$$ \begin{align*} \widehat{u}_{j}(x):= \begin{cases} u_{d_{j} }(x)& \, \text{in } \mathbb{R}^{n}_{+}, \\ u_{d_{j} }(x', -x_{n}) & \, \text{in } \mathbb{R}^{n}_{-}, \end{cases} \end{align*} $$

where

$$ \begin{align*}x'=(x_{1},x_{2},\ldots, x_{n-1}),\quad \mathbb{R}^{n}_{+}=\{(x',x_{n}) \mid x_{n} \geq 0 \},\,\,\mathbb{R}^{n}_{-}=\{(x',x_{n}) \mid x_{n} \leq 0 \}. \end{align*} $$

Also, define a scaled function

(5-13) $$ \begin{align} \psi_{j}(y):=\widehat{u}_{j}(yd_{j}^{{1}/{2s}}+z_{j})\quad\text{for } y \in \mathbb{R}^{n}. \end{align} $$

Now, for $z_{j}=(z_{j}^{\prime },z_{jn}),$ we can write $z_{jn}=\alpha _{j}d_{j}^{{1}/{2s}}$ for some $\alpha _{j}>0.$ The sequence $\{\alpha _{j} \} $ is bounded, which follows from Lemma 1.4. Let

$$ \begin{align*} \rho_{j}:=\frac{\rho(z_{j}, \partial \Omega)}{d_{j}^{{1}/{2s}}} , \end{align*} $$

where $\rho (z_{j}, \partial \Omega )$ denotes the distance between $z_{j}$ and $ \partial \Omega .$ One can see easily that the function $\psi _{j}$ satisfies the equation

$$ \begin{align*} (-\Delta)^{s}\psi_{j}(y)+ \psi_{j}(y)= \psi_{j}(y)^{p}+ d_{j}{h}(y) \quad \text{in } B_{\rho_{j}} \end{align*} $$

for some function ${h}$ of $y.$ To see this, let $y \in B_{\rho _{j}}$ , so

(5-14) $$ \begin{align} (-\Delta)^{s}\psi_{j}(y)&=c_{n,s}\ \mathrm{PV} \int_{\mathbb{R}^{n}}\frac{\psi_{j}(y)-\psi_{j}(x)}{\vert y-x\vert^{n+2s}}\,dx= c_{n,s} \lim_{\epsilon \rightarrow 0} \int_{\mathcal{C} B_{\epsilon}(y)}\frac{\psi_{j}(y)-\psi_{j}(x)}{\vert y-x\vert^{n+2s}}\,dx \nonumber \\ &= c_{n,s} \lim_{\epsilon \rightarrow 0} \bigg[ \int_{\mathcal{C} B_{\epsilon}(y)}\frac{\widehat{u}_{j}(yd_{j}^{{1}/{2s}}+z_{j})-\widehat{u}_{j}(xd_{j}^{{1}/{2s}}+z_{j})}{\vert y-x\vert^{n+2s}}\,dx \bigg] \nonumber \\ &= c_{n,s} \lim_{\epsilon \rightarrow 0} \int_{\{x_{n} \geq -\alpha_{j}\}\bigcap \mathcal{C} B_{\epsilon}(y)}\frac{\widehat{u}_{j}(yd_{j}^{{1}/{2s}}+z_{j})-\widehat{u}_{j}(xd_{j}^{{1}/{2s}}+z_{j})}{\vert y-x\vert^{n+2s}}\,dx \nonumber \\ & \quad+ c_{n,s} \lim_{\epsilon \rightarrow 0} \int_{\{x_{n} \leq-\alpha_{j}\}\bigcap \mathcal{C}B_{\epsilon}(y)}\frac{\widehat{u}_{j}(yd_{j}^{{1}/{2s}}+z_{j})-\widehat{u}_{j}(xd_{j}^{{1}/{2s}}+z_{j})}{\vert y-x\vert^{n+2s}}\,dx. \end{align} $$

For $y_{n} \geq -\alpha _{j},$

$$ \begin{align*} &(-\Delta)^{s}\psi_{j}(y)\nonumber\\&= c_{n,s}\lim_{\epsilon \rightarrow 0} \int_{\{x_{n} \geq -\alpha_{j}\}\bigcap \mathcal{C} B_{\epsilon}(y)}\frac{{u}_{{j}}(yd_{j}^{{1}/{2s}}+z_{j})-{u}_{{j}}(xd_{j}^{{1}/{2s}}+z_{j})}{\vert y-x\vert^{n+2s}}\,dx \nonumber \\& \quad+ c_{n,s}\lim_{\epsilon \rightarrow 0} \int_{\{x_{n} \leq-\alpha_{j}\}\bigcap \mathcal{C} B_{\epsilon}(y)}\frac{{u}_{{j}}(yd_{j}^{{1}/{2s}}+z_{j})-{u}_{{j}}(x' d_{j}^{{1}/{2s}}+z_{j}^{\prime}, -(x_{n}+\alpha_{j}d_{j}^{{1}/{2s}}))}{\vert y-x\vert^{n+2s}}\,dx \nonumber \\&= c_{n,s} \lim_{\epsilon \rightarrow 0} \int_{\{x_{n} \geq -\alpha_{j}\} \bigcap \mathcal{C} B_{\epsilon}(y)}\frac{{u}_{{j}}(yd_{j}^{{1}/{2s}}+z_{j})-{u}_{{j}}(xd_{j}^{{1}/{2s}}+z_{j})}{\vert y-x\vert^{n+2s}}\,dx \nonumber \\&\quad + c_{n,s}\lim_{\epsilon \rightarrow 0} \int_{\{x_{n} \leq-\alpha_{j}\}\bigcap \mathcal{C} B_{\epsilon}(y)}\frac{{u}_{{j}}(yd_{j}^{{1}/{2s}}+z_{j})-{u}_{{j}}(x'd_{j}^{{1}/{2s}}+z_{j}^{\prime}, -(x_{n}+\alpha_{j}d_{j}^{{1}/{2s}}))}{\vert y-x\vert^{n+2s}}\,dx \nonumber \\&= c_{n,s} \lim_{\epsilon \rightarrow 0} \int_{\mathcal{C} B_{\epsilon}(y)}\frac{{u}_{{j}}(yd_{j}^{{1}/{2s}}+z_{j})-{u}_{{j}}(xd_{j}^{{1}/{2s}}+z_{j})}{\vert y-x\vert^{n+2s}}\,dx \nonumber \\&\quad + c_{n,s}\lim_{\epsilon \rightarrow 0} \int_{\{x_{n} \leq-\alpha_{j}\} \bigcap \mathcal{C}B_{\epsilon}(y)}\frac{{u}_{{j}}(xd_{j}^{{1}/{2s}}+z_{j}) -{u}_{{j}}(x'd_{j}^{{1}/{2s}}+z_{j}^{\prime}, -(x_{n}+\alpha_{j}d_{j}^{{1}/{2s}}))}{\vert y-x\vert^{n+2s}}\,dx \nonumber \\&= c_{n,s} \lim_{\epsilon \rightarrow 0} \int_{\mathcal{C} B_{\epsilon}(y)}\frac{{u}_{{j}}(yd_{j}^{{1}/{2s}}+z_{j})-{u}_{{j}}(xd_{j}^{{1}/{2s}}+z_{j})}{\vert y-x\vert^{n+2s}}\,dx\nonumber\\&\quad + c_{n,s}\lim_{\epsilon \rightarrow 0} \int_{\{x_{n} \leq-\alpha_{j}\}\bigcap \mathcal{C} B_{\epsilon}(y)}\frac{{u}_{{j}}(xd_{j}^{{1}/{2s}}+z_{j}) -\widehat{u}_{{j}}(xd_{j}^{{1}/{2s}}+z_{j})}{\vert y-x\vert^{n+2s}}\,dx . \end{align*} $$

Making the change of variables

$$ \begin{align*}yd_{j}^{{1}/{2s}}+z_{j}=a \text{ and } xd_{j}^{{1}/{2s}}+z_{j}=b,\end{align*} $$

we get

(5-15) $$ \begin{align} (-\Delta)^{s}\psi_{j}(y)&= d_{j}(-\Delta)^{s}u_{j}(a)+ d_{j} c_{n,s} \lim_{\eta \rightarrow 0} \int_{\{b_{n} \leq 0\} \bigcap \mathcal{C} B_{\eta }(a)}\frac{{u}_{{j}}(b) -\widehat{u}_{{j}}(b)}{\vert a-b\vert^{n+2s}}db \nonumber\\ &= d_{j}(-\Delta)^{s}u_{j}(a)+ d_{j}h(a), \end{align} $$

where

$$ \begin{align*}\eta = \epsilon d_{j}^{{1}/{2s}} \end{align*} $$

and

$$ \begin{align*}h(a)= c_{n,s} \lim_{\eta \rightarrow 0} \int_{\{b_{n} \leq 0\} \bigcap \mathcal{C} B_{\eta }(a)}\frac{{u}_{{j}}(b) -\widehat{u}_{{j}}(b)}{\vert a-b\vert^{n+2s}}\,db.\end{align*} $$

Note that $a \in \Omega .$

Now, consider the case $y_{n} \leq -\alpha _{j}.$ Equation (5-14) becomes

$$ \begin{align*} &(-\Delta)^{s}\psi_{j}(y)= I_1 + I_2 \end{align*} $$

where

$$ \begin{align*}&I_1 = \int_{\{x_{n} \geq -\alpha_{j}\}\bigcap \mathcal{C} B_{\epsilon}(y)}\frac{{u}_{j}(y' d_{j}^{{1}/{2s}}+z_{j}^{\prime}, -(y_{n}d_{j}^{{1}/{2s}}+\alpha_{j}d_{j}^{{1}/{2s}}))-{u}_{j}(xd_{j}^{{1}/{2s}}+z_{j})}{\vert y-x\vert^{n+2s}}\,dx \end{align*} $$

and

(5-16) $$ \begin{align} &I_2 = \int_{\{x_{n} \leq-\alpha_{j}\}\bigcap \mathcal{C} B_{\epsilon}(y)}\frac{{u}_{j}(y' d_{j}^{{1}/{2s}}+z_{j}^{\prime}, -(y_{n}d_{j}^{{1}/{2s}}+\alpha_{j}d_{j}^{{1}/{2s}}))- {u}_{j}(x' d_{j}^{{1}/{2s}}+z_{j}^{\prime}, -(x_{n}d_{j}^{{1}/{2s}}+\alpha_{j}d_{j}^{{1}/{2s}}))}{\vert y-x\vert^{n+2s}}\,dx \end{align} $$

Let us introduce some notation. We write $\widehat {x}= (x',-x_{n})$ , $\widetilde {x}=(\widehat {x}',\widehat {x}_{n})$ and $\widehat {x}_{n}=-x_{n}$ for $x=(x',x_{n}) \in \mathbb {R}^{n}, n>1.$ Using these, let us compute

$$ \begin{align*} I_{2}&= c_{n,s} \lim_{\epsilon \rightarrow 0} \bigg[\int_{\{\widehat{x}_{n} \geq \alpha_{j}\} \bigcap \mathcal{C} B_{\epsilon}(\widehat{y})}\frac{{u}_{j}(\widehat{y}' d_{j}^{{1}/{2s}}+\hat{z}_{j}^{\prime}, \widehat{y}_{n}d_{j}^{{1}/{2s}}+\widehat{\alpha}_{j}d_{j}^{{1}/{2s}})- {u}_{j}(\widehat{x}' d_{j}^{{1}/{2s}}+\widehat{z}_{j}^{\prime}, \widehat{x}_{n}d_{j}^{{1}/{2s}}+\widehat{\alpha}_{j}d_{j}^{{1}/{2s}})}{\vert\widehat{y}-\widehat{x}\vert^{n+2s}}d\widetilde{x} \bigg] \nonumber \\ &= c_{n,s} \lim_{\epsilon \rightarrow 0} \bigg[\int_{\{\widehat{x}_{n} \geq \alpha_{j}\} \bigcap \mathcal{C} B_{\epsilon}(\widehat{y})}\frac{{u}_{j}(\widetilde{y}d_{j}^{{1}/{2s}}+\widetilde{z}_{j})- {u}_{j}(\widetilde{x}d_{j}^{{1}/{2s}}+\widetilde{z}_{j} )}{\vert\widehat{y}-\widehat{x}\vert^{n+2s}}d\widetilde{x} \bigg] \nonumber\\ &= c_{n,s} \lim_{\epsilon \rightarrow 0} \bigg[\int_{\{\widehat{x}_{n} \geq \alpha_{j}\} \bigcap \mathcal{C} B_{\epsilon}(\widetilde{y})}\frac{{u}_{j}(\widetilde{y}d_{j}^{{1}/{2s}}+\widetilde{z}_{j})- {u}_{j}(\widetilde{x}d_{j}^{{1}/{2s}}+\widetilde{z}_{j} )}{\vert\widetilde{y}-\widetilde{x}\vert^{n+2s}}d\widetilde{x} \bigg]. \end{align*} $$

Now, we simplify $I_{1}$ :

$$ \begin{align*} I_{1}&= c_{n,s} \lim_{\epsilon \rightarrow 0} \bigg[ \int_{\{x_{n} \geq -\alpha_{j}\} \bigcap \mathcal{C} B_{\epsilon}({y})}\!\!\frac{{u}_{j}(y' d_{j}^{{1}/{2s}}+z_{j}^{\prime}, -(y_{n}d_{j}^{{1}/{2s}}+\alpha_{j}d_{j}^{{1}/{2s}}))- {u}_{j}(x' d_{j}^{{1}/{2s}}+z_{j}^{\prime}, -(x_{n}d_{j}^{{1}/{2s}}+\alpha_{j}d_{j}^{{1}/{2s}}))}{\vert y-x\vert^{n+2s}} \nonumber \\ & \quad+ \int_{\{x_{n} \geq -\alpha_{j}\} \cap \mathcal{C} B_{\epsilon}({y})} \frac{ {u}_{j}(w'd_{j}^{{1}/{2s}}+z_{j}^{\prime}, -(x_{n}d_{j}^{{1}/{2s}}+\alpha_{j}d_{j}^{{1}/{2s}}))-{u}_{j}(xd_{j}^{{1}/{2s}}+z_{j})}{\vert y-x\vert^{n+2s}}\,dx \bigg] \nonumber \\ &= c_{n,s}\lim_{\epsilon \rightarrow 0} \bigg[ \int_{\{\widehat{x}_{n} \leq \alpha_{j}\} \bigcap \mathcal{C}B_{\epsilon}(\widetilde{y})}\frac{{u}_{j}(\widetilde{y}d_{j}^{{1}/{2s}}+\widetilde{z}_{j})- {u}_{j}(\widetilde{x}d_{j}^{{1}/{2s}}+\widetilde{z}_{j} )}{\vert\widetilde{y}-\widetilde{x}\vert^{n+2s}}d\widetilde{x}\nonumber\\ &\quad+ \int_{\{{x}_{n} \geq -\alpha_{j}\} \cap \mathcal{C}B_{\epsilon}(\widetilde{y})}\frac{{u}_{j}(\widetilde{x}d_{j}^{{1}/{2s}}+\widetilde{z}_{j})- \widehat{{u}}_{j}(\widetilde{x}d_{j}^{{1}/{2s}}+\widetilde{z}_{j} )}{\vert\widetilde{y}-\widetilde{x}\vert^{n+2s}}d\widetilde{x} \bigg]. \end{align*} $$

Using these estimates for $I_{1}$ and $I_{2}$ in (5-16),

$$ \begin{align*} (-\Delta)^{s}\psi_{j}(y)&= c_{n,s}\ \mathrm{PV} \int_{\mathbb{R}^{n}}\frac{{u}_{j}(\widetilde{y}d_{j}^{{1}/{2s}}+\widetilde{z}_{j})- {u}_{j}(\widetilde{x}d_{j}^{{1}/{2s}}+\widetilde{z}_{j} )}{\vert\widetilde{y}-\widetilde{x}\vert^{n+2s}}d\widetilde{x}\nonumber\\ &\quad+ c_{n,s} \lim_{\epsilon \rightarrow 0} \int_{\{{x}_{n} \geq -\alpha_{j}\} \bigcap \mathcal{C}B_{\epsilon}(\widetilde{y})}\frac{{u}_{j}(\widetilde{x}d_{j}^{{1}/{2s}}+\widetilde{z}_{j})- \widehat{{u}}_{j}(\widetilde{x}d_{j}^{{1}/{2s}}+\widetilde{z}_{j} )}{\vert\widetilde{y}-\widetilde{x}\vert^{n+2s}}d\widetilde{x}. \end{align*} $$

By the change of variables

$$ \begin{align*}\widetilde{y}d_{j}^{{1}/{2s}}+\widetilde{z}_{j}=e \quad\text{and}\quad \widetilde{w}d_{j}^{{1}/{2s}}+\widetilde{z}_{j}=f,\end{align*} $$

we get

(5-17) $$ \begin{align} &(-\Delta)^{s}\psi_{j}(y)= d_{j}(-\Delta)^{s}u_{j}(e)\nonumber\\ &\qquad+ d_{j} c_{n,s} \lim_{\eta \rightarrow 0} \int_{\{f_{n} \leq 0\}\bigcap \mathcal{C}B_{\eta}(e)}\frac{{u}_{{j}}(f) -\widehat{u}_{{j}}(f)}{\vert e-f\vert^{n+2s}}\,df, \,\mbox{where} f_n \mbox{ is the } n\,\mbox{th coordinate of } f \nonumber \\ &\quad= d_{j}(-\Delta)^{s}u_{j}(e) + d_{j}h(e). \end{align} $$

Note that $e \in \Omega .$ Further, for $y \in B_{\rho _{j}},$

$$ \begin{align*} \psi_{j}(y)= \widehat{u}_{j}(yd_{j}^{{1}/{2s}}+ z_{j})= \begin{cases} u_{d_{j} }(yd_{j}^{{1}/{2s}}+z_{j})& \text{if } y_{n} \geq - \alpha_{j}, \\ u_{d_{j} }(y' d_{j}^{{1}/{2s}}+z_{j}^{\prime}, -(y_{n}d_{j}^{{1}/{2s}}+ \alpha_{j}d_{j}^{{1}/{2s}})) & \text{if } y_{n} \leq -\alpha_{j}. \end{cases} \end{align*} $$

We can write

$$ \begin{align*}(y' d_{j}^{{1}/{2s}}+z_{j}^{\prime}, -(y_{n}d_{j}^{{1}/{2s}}+ \alpha_{j}d_{j}^{{1}/{2s}}))=\widetilde{y}d_{j}^{{1}/{2s}}+\widetilde{z}_{j}.\end{align*} $$

Again re-naming the variables $yd_{j}^{{1}/{2s}}+ z_{j}$ and $\widetilde {y}d_{j}^{{1}/{2s}}+\widetilde {z}_{j}$ by a and $e,$ respectively,

$$ \begin{align*} \psi_{j}(y)= \begin{cases} u_{d_{j} }(a)& \text{if } y_{n} \geq -\alpha_{j}, \\ u_{d_{j} }(e) & \text{if } y_{n} \leq -\alpha_{j}. \end{cases} \end{align*} $$

We know that $u_{j}$ satisfies (1-1) in the point-wise sense as well. Therefore, combining above equation with (5-15), (5-17), we have for $y \in B_{\rho _{j}}, $

$$ \begin{align*} (-\Delta)^{s}\psi_{j}(y)+\psi_{j}(y)=\psi_{j}(y)^{p}+ d_{j}{h}(y). \end{align*} $$

Now, arguing as in the proof of Step I with minor modifications, one can obtain a convergent subsequence of $\{\psi _{j} \},$ which we denote again by $\{\psi _{j} \}$ such that $\psi _{j} \rightarrow v$ in $C_{loc}^{2}(\mathbb {R}^{n}).$ Therefore, as $d_{j}\downarrow 0,$

$$ \begin{align*} (-\Delta)^{s}v+ v= v^{p}\quad \text{in } \mathbb{R}^{n}. \end{align*} $$

Since $v \in H^{s}(\mathbb {R}^{n})$ and v is radially decreasing, v is spherically symmetric to $y=0.$ Moreover, v has power-type decay at infinity, which follows from Theorem 2.8, that is,

$$ \begin{align*} v(r) \leq \frac{C_{2}}{r^{n+2s}}, \quad r \geq 1, \end{align*} $$

for some constant $C_{2}>0.$ Let us define $\delta _{R}$ as in (5-7), that is,

$$ \begin{align*}\delta_{R}:= \frac{C_{2}}{R^{n+2s}}\end{align*} $$

for R sufficiently large to be defined later. Then, there exists an integer $j_{R}$ such that for $j \geq j_{R},$

(5-18) $$ \begin{align} \Vert\psi_{j}-v\Vert_{C^{2}(\overline{B_{4R}})} \leq \delta_{R}. \end{align} $$

We choose R sufficiently large that $R> \alpha _{j}$ for all $j,$ where the $\alpha _{j}$ terms are the same as defined earlier right after (5-13). We can choose such an R because $\{\alpha _{j}\}$ is a bounded sequence. The following lemma is very useful to prove our claim that $z_{d} \in \partial \Omega .$

Lemma 5.2 (see [Reference Ni and Takagi35, Lemma 4.2])

Let $f \in C^{2}(\overline {B_{t}})$ be a radial function. Assume that f satisfies $f'(0)=0$ and $f"(r)<0$ for $0 \leq r \leq t.$ Then, there exists a $\eta> 0$ such that if $g \in C^{2}(\overline {B_{t}}) $ satisfies:

  1. (1) $\nabla g(0)=0$ ;

  2. (2) $ \Vert f-g\Vert _{C^{2}(\overline {B_{t}})}< \eta ,$

then $\nabla g \neq 0$ for $x \neq 0.$

Now, we use this lemma to show that $\psi _{j}$ has only one local maximum point in $B_{R}.$ For this, we choose two numbers $k,l$ $(0<k<l)$ such that $v"(r)<0 $ for $0 \leq r \leq k.$ Further, we see that $v"(0)<0$ and $ v(k)<1.$ Let us define

$$ \begin{align*} \theta = \min \{ \vert v'(r)\vert \mid k \leq r \leq l \}. \end{align*} $$

It is easy to observe that $\theta>0$ because $v'<0$ for $r>0.$ Then for $\delta _{R}<\theta ,$ we have by (5-18) that

$$ \begin{align*} 0< \theta - \delta_{R} \leq \vert\nabla v(y)\vert -\vert\nabla \psi_{j}(y)-\nabla v(y)\vert \leq \vert\nabla \psi_{j}(y)\vert \text{ for } k \leq \vert y\vert \leq l. \end{align*} $$

Applying Lemma 5.2 in the ball $\overline {B}_{k},$ we conclude that $y=0$ is the only local maximum point of $\psi _{j}$ in $B_{l}.$ If $y_{j}$ is a maximum point of $\psi _{j}$ in $B_{R},$ then by Lemma 3.8, we have $\psi _{j} \geq 1.$ Choose $R>0$ sufficiently large so that $\delta _{R}< 1-v(l).$ Therefore,

$$ \begin{align*} \psi_{j}(y) \leq v(y) + \delta_{R} \leq v(l)+ \delta_{R}<1. \end{align*} $$

Hence, $y_{j} \in B_{l}$ and therefore $y_{j}=0.$

If $\alpha _{j}>0,$ then by the definition of $\widehat {u}_{j}$ , $z_{R}^{*}=(z_{j}^{\prime }, -\alpha _{j}d_{j}^{{1}/{2s}})$ is also a maximum point of $\widehat {u}_{j}.$ This implies that $(0,-\alpha _{j})$ is another maximum point of $\psi _{j}$ in $B_{R},$ which is a contradiction. This proves our claim and hence completes the proof of Theorem 1.4.

Appendix A

Proof of (3-8)

For real numbers $x,y \geq 0$ and $k \geq 1,$ we show that

$$ \begin{align*} \frac{1}{k}(x^{k}-y^{k})^{2}\leq (x-y)(x^{2k-1}-y^{2k-1}). \end{align*} $$

Clearly, the inequality holds when either x or y or both are zero or $x=y$ . Thus, without loss of generality, we may assume that $x>y>0.$ Now, our claim is reduced to showing that

$$ \begin{align*} \frac{1}{k} \bigg(1- \bigg(\frac{y}{x}\bigg)^k \bigg)^2 \leq \bigg( 1- \frac{y}{x}\bigg) \bigg(1- \bigg(\frac{y}{x}\bigg)^{2k-1}\bigg),\end{align*} $$

that is, to show that

$$ \begin{align*}(1-a^k)^2 \leq k (1-a)(1-a^{2k-1}),\end{align*} $$

where $0<a:= \frac {y}{x}<1.$ Consider

$$ \begin{align*} f(a)&:= k (1-a)(1-a^{2k-1})- (1-a^k)^{2} \\ & \geq (1-a^k) (k(1-a)- (1-a^k) )\\ & \geq (1-a^k)(1-a) (k-(1+a+a^2+\cdots + a^{k-1}) )\\ & \geq (1-a^k)(1-a) (k-k) =0. \end{align*} $$

This proves the inequality.

Acknowledgements

The authors thank the referee for their useful comments. S.G. thanks CSIR for the financial support under grant 09/1031(0009)/2019-EMR-I. J.T. thanks DST/SERB for the financial support under grant no. CRG/2020/000041.

Footnotes

Communicated by Florica C. Cîrstea

References

Adimurthi, and Mancini, G., ‘The Neumann problem for elliptic equations with critical non-linearity. A tribute in honour of G, Prodi’, Ann. Sc. Norm. Super. Pisa Cl. Sci. (5) 1 (1991), 0925.Google Scholar
Adimurthi, , Pacella, F. and Yadava, S. L., ‘Interaction between the geometry of the boundary and positive solutions of a semilinear Neumann problem with critical nonlinearity’, J. Funct. Anal. 113 (1993), 318350.Google Scholar
Arumugam, G. and Tyagi, J., ‘Keller–Segel chemotaxis models: a review’, Acta Appl. Math. 171 (2021), Paper no. 6, 82 pages.Google Scholar
Barrios, B., Montoro, L., Peral, I. and Soria, F., ‘Neumann conditions for the higher order $s$ -fractional Laplacian ${\left(-\varDelta \right)}^s$ with $s>1$ ’, Nonlinear Anal. 193 (2020), Paper no. 111368, 34 pages.1$+’,+Nonlinear+Anal.+193+(2020),+Paper+no.+111368,+34+pages.>Google Scholar
Bartumeus, F., Peters, F., Pueyo, S., Marrasé, C. and Catalan, J., ‘Helical Lévy walks: adjusting searching statistics to resource availability in microzooplankton’, Proc. Natl. Acad. Sci. USA 100 (2003), 15811633.Google Scholar
Biagi, S., Dipierro, S., Valdinoci, E. and Vecchi, E., ‘Mixed local and nonlocal elliptic operators: regularity and maximum principles’, Comm. Partial Differential Equations 47(3) (2022), 585629.Google Scholar
Chen, G., ‘Singularly perturbed Neumann problem for fractional Schrödinger equations’, Sci. China Math. 61(4) (2018), 695708.Google Scholar
Chen, J. and Gao, Z., ‘Ground state solutions for fractional Schrödinger equation with variable potential and Berestycki–Lions type nonlinearity’, Bound. Value Probl. 2019 (2019), Paper no. 148, 24 pages.Google Scholar
Choi, W., Kim, S. and Lee, K.-A., ‘Asymptotic behavior of solutions for nonlinear elliptic problems with the fractional Laplacian’, J. Funct. Anal. 266(11) (2014), 65316598.Google Scholar
Cinti, E. and Colasuonno, F., ‘A nonlocal supercritical Neumann problem’, J. Differential Equations 268 (2020), 22462279.Google Scholar
Cinti, E. and Colasuonno, F., ‘Existence and non-existence results for a semilinear fractional Neumann problem’, NoDEA Nonlinear Differential Equations Appl. 30(6) (2023), Paper no. 79, 20 pages.Google Scholar
Di Nezza, E., Palatucci, G. and Valdinoci, E., ‘Hitchhiker’s guide to the fractional Sobolev spaces’, Bull. Sci. Math. 136(5) (2012), 521573.Google Scholar
Dipierro, S., Palatucci, G. and Valdinoci, E., ‘Existence and symmetry results for a Schrödinger type problem involving the fractional Laplacian’, Matematiche (Catania) 68(1) (2013), 201216.Google Scholar
Dipierro, S., Ros-Oton, X. and Valdinoci, E., ‘Nonlocal problems with Neumann boundary conditions’, Rev. Mat. Iberoam. 33(2) (2017), 377416.Google Scholar
Dipierro, S., Soave, N. and Valdinoci, E., ‘On fractional elliptic equations in Lipschitz sets and epigraphs: regularity, monotonicity and rigidity results’, Math. Ann. 369(3–4) (2017), 12831326.Google Scholar
Dipierro, S. and Valdinoci, E., ‘Description of an ecological niche for a mixed local/nonlocal dispersal: an evolution equation and a new Neumann condition arising from the superposition of Brownian and Lévy processes’, Phys. A 575 (2021), Paper no. 126052, 20 pages.Google Scholar
Du, X., Jin, T., Xiong, J. and Yang, H., ‘Blow up limits of the fractional Laplacian and their applications to the fractional Nirenberg problem’, Proc. Amer. Math. Soc. 151(11) (2023), 46934701.Google Scholar
Escudero, C., ‘The fractional Keller–Segel model’, Nonlinearity 19 (2006), 29092918.Google Scholar
Fall, M. M., ‘Regularity results for nonlocal equations and applications’, Calc. Var. Partial Differential Equations 59 (2020), 181.Google Scholar
Felmer, P. and Quaas, A., ‘Positive solutions of the nonlinear Schrödinger equation with the fractional Laplacian’, Proc. Roy. Soc. Edinburgh Sect. A 142(6) (2012), 12371262.Google Scholar
Felmer, P. and Wang, Y., ‘Radial symmetry of positive solutions to equations involving the fractional Laplacian’, Commun. Contemp. Math. 16(1) (2014), Paper no. 1350023, 24 pages.Google Scholar
Gandal, S. and Tyagi, J., ‘The Neumann problem for a class of semilinear fractional equations with critical exponent’, Bull. Sci. Math. 188 (2023), Paper no. 103322, 35 pages.Google Scholar
He, X., Rădulescu, V. D. and Zou, W., ‘Normalized ground states for the critical fractional Choquard equation with a local perturbation’, J. Geom. Anal. 32(10) (2022), Paper no. 252, 51 pages.Google Scholar
Horstmann, D., ‘From 1970 until present: the Keller–Segel model in chemotaxis and its consequences I’, Jahresber. Dtsch. Math.-Ver. 105 (2003), 103165.Google Scholar
Horstmann, D., ‘From 1970 until present: the Keller–Segel model in chemotaxis and its consequences II’, Jahresber. Dtsch. Math.-Ver. 106 (2004), 5169.Google Scholar
Huang, H. and Liu, J., ‘Well-posedness for the Keller–Segel equation with fractional Laplacian and the theory of propagation of chaos’, Kinet. Relat. Models 9 (2016), 715748.Google Scholar
Kabeya, Y. and Ni, W.-M., ‘Stationary Keller–Segel model with the linear sensitivity’, RIMS K $\check{o}$ ky $\check{u}$ roku Bessatsu 1025 (1998), 4465.Google Scholar
Keller, E. F. and Segel, L. A., ‘Initiation of slime mold aggregation viewed as an instability’, J. Theoret. Biol. 26 (1970), 399415.Google Scholar
Levandowsky, M., White, B. S. and Schuste, F. L., ‘Random movements of soil amebas’, Acta Protozool 36 (1997), 237248.Google Scholar
Lin, C. S. and Ni, W.-M., ‘On the diffusion coefficient of a semilinear Neumann problem’, in: Calculus of Variations and Partial Differential Equations, Lecture Notes in Mathematics, 1340 (eds. Hildebrandt, S., Kinderlehrer, D. and Miranda, M.) (Springer, New York–Berlin, 1986).Google Scholar
Lin, C. S., Ni, W.-M. and Takagi, I., ‘Large amplitude stationary solutions to a chemotaxis system’, J. Differential Equations 72 (1988), 127.Google Scholar
Molica Bisci, G., Rădulescu, V. D. and Servadei, R., Variational Methods for Nonlocal Fractional Problems, Encyclopedia of Mathematics and its Applications, 162 (Cambridge University Press, Cambridge, 2016).Google Scholar
Mugnai, D., Perera, K. and Proietti Lippi, E., ‘A priori estimates for the fractional $p$ -Laplacian with nonlocal Neumann boundary conditions and applications’, Commun. Pure Appl. Anal. 21(1) (2022), 275292.Google Scholar
Ni, W.-M. and Takagi, I., ‘On the existence and shape of solutions to a semilinear Neumann problem’, in: Proceedings of the Conference on Nonlinear Diffusion Equations and their Equilibrium States, 3, Gregynog (eds. Lloyd, N. G., Ni, W. M., Peletier, L. A. and Serrin, J.) (Birkhäuser, Boston, MA, 1989), 425436.Google Scholar
Ni, W.-M. and Takagi, I., ‘On the shape of least energy solutions to a semilinear Neumann problem’, Comm. Pure Appl. Math. 44 (1991), 819851.Google Scholar
Ros-Oton, X. and Serra, J., ‘The Dirichlet problem for the fractional Laplacian: regularity up to the boundary’, J. Math. Pures Appl. (9) 101 (2012), 275302.Google Scholar
Secchi, S., ‘On fractional Schrödinger equations in ${\mathbb{R}}^n$ without the Ambrosetti–Rabinowitz condition’, Topol. Methods Nonlinear Anal. 47(1) (2016), 1941.Google Scholar
Servadei, R. and Valdinoci, E., ‘Mountain pass solutions for non-local elliptic operators’, J. Math. Anal. Appl. 389(2) (2012), 887898.Google Scholar
Servadei, R. and Valdinoci, E., ‘The Brezis–Nirenberg result for the fractional Laplacian’, Trans. Amer. Math. Soc. 367(1) (2015), 67102.Google Scholar