Abstract
We consider positive weak solutions to \((-\Delta )^s u=f(x,u)\) in \(\Omega {\setminus } \Gamma \) under zero Dirichlet boundary condition. The domain \(\Omega \) is bounded or is the whole space, and the solution has a singularity on the singular set \(\Gamma \). Under suitable assumptions on f we prove symmetry and monotonicity properties of the solutions when the singular set \(\Gamma \) has zero s-capacity.
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1 Introduction
In this paper we study the following nonlocal semilinear elliptic problem:
where \(0<s<1,\, N>2s\) and \(\Omega \) is a bounded domain with smooth boundary \(\partial \Omega \), or it is the whole space \({\mathbb {R}}^N\). Note that the equation is satisfied in \(\Omega {\setminus } \Gamma \), where the set \(\Gamma \subset \Omega \), which is referred to as the singular set, is compact and has zero s-capacity (see Sect. 2 below). We consider solutions belonging to \(W^{s,2}_{\text {loc}}({\mathbb {R}}^N{\setminus }\Gamma )\cap L^{1}({\mathbb {R}}^N)\cap C({\mathbb {R}}^N{\setminus }\Gamma )\), and the equation is understood in the weak distributional sense, see Definition 2.2 below. As it is customary, in the case of a bounded domain \(\Omega \), the Dirichlet datum is expressed by the fact that u is identically zero outside \(\Omega \).
We study symmetry and monotonicity properties of solutions via the moving plane method that was introduced in [2, 22], and in particular we refer to the celebrated papers [4, 15] where it was firstly exploited to study symmetry and monotonicity properties of the solutions.
Here we deal with singular solutions in the nonlocal case; for the local case we refer to [6, 21, 23, 28]. Symmetry results, when \(\Gamma =\emptyset \), for equations involving the fractional Laplacian via the moving plane method, for more regular problems, can be found for instance in [3, 12, 16, 17] and also in [7, 8, 12, 14, 20]. Other works, for the case \(\Gamma =\emptyset \) and in the nonlocal framework, that study the symmetry of solutions using other techniques are, for example, [5, 11, 24].
In our results we shall assume in the case of a bounded domain \(\Omega \) that the nonlinearity f is uniformly locally Lipschitz continuous far from the singular set \(\Gamma \). More precisely we make the following assumption:
(\(A_f^1\)). For any \(0\le \tau ,t\le M\) and for any compact set \(K\subset \Omega {\setminus }\Gamma \), there exists a positive constant \(C=C(K,M)\) such that
Furthermore, \(f(\cdot ,\tau )\) is nondecreasing in the \(x_1\) -direction in \(\Omega \cap \{x_1<0\}\) and symmetric with respect to the hyperplane \(\{x_1=0\}\).
In this setting our main result is the following
Theorem 1.1
Let \(u\in W^{s,2}_\mathrm{{loc}}({\mathbb {R}}^N{\setminus }\Gamma )\cap L^{1}({\mathbb {R}}^N)\cap C({\mathbb {R}}^N{\setminus } \Gamma )\) be a solution to (1.1) with f fulfilling \((A_f^1)\). Assume that the singular set \(\Gamma \subset \Omega \) is compact and has zero s-capacity.
If \(\Omega \) is convex and symmetric in the \(x_1\)-direction and \(\Gamma \subset \{x_1=0\}\), then u is symmetric with respect to the hyperplane \(\{x_1=0\}\) and increasing in the \(x_1\)-direction in \(\Omega \cap \{x_1<0\}\).
If the domain is a ball and \(\Gamma \) is the center of the ball, then the solution is radial and radially decreasing about the center of the ball.
The proof exploits a new technique based also on some ideas introduced in [23] for the local case. The nonlocal case exhibits many peculiarities related in particular to the notion of solution and to the fact that the critical set plays a role also far from it, because of the nonlocal nature of the operator.
In the second part of the paper we consider problem (1.1), with \(f=f(u)\) in the whole space \({\mathbb {R}}^N\), that is we consider
with \(f(\cdot )\) satisfying a critical growth assumption, namely:
(\(A_f^2\)) f is \(C^1\) and convex with \(f(0)=0\) and, for any \(t>0\)
for some \(C_f>0\), where \(2^*_s=2N/(N-2s), N>2s\) is the Sobolev critical exponent. We dropped the dependence of f on x to avoid further technicalities.
In this setting our main result is the following
Theorem 1.2
Let \(u\in W^{s,2}_\mathrm{{loc}}({\mathbb {R}}^N{\setminus }\Gamma )\cap L^{1}({\mathbb {R}}^N)\cap C({\mathbb {R}}^N{\setminus } \Gamma )\) be a solution to (1.2) with f fulfilling \((A_f^2)\). Assume that the singular set \(\Gamma \subset {\mathbb {R}}^N\) is compact and has zero s-capacity.
If for some \(R_0>0\), \(\Gamma \subset \{x_1=0\}\cap B_{R_0} \) and \(u\in L^{2^*_s}({\mathbb {R}}^N{\setminus } B_{R_0})\), then u is symmetric with respect to the hyperplane \(\{x_1=0\}\) and increasing in the \(x_1\)-direction in \(\{x_1<0\}\).
If u has only a nonremovable singularity at the origin, then the solution is radial and radially decreasing about the origin.
In the local case the problem in the whole space can be studied in a similar way as in the case of a bounded domain. This is not the case when considering nonlocal problems; indeed, a fine density argument and new estimates are required.
The paper is organized as follows: we collect some preliminary results in Sect. 2. The case of a bounded domain, namely Theorem 1.1, is studied in Sect. 3. In Sect. 4 we deal with the case of the whole space and we prove Theorem 1.2.
2 Notations and preliminary results
Let us recall that, given a function u in the Schwartz’s class \({\mathcal {S}}({\mathbb {R}}^{N})\) we define for \(0<s<1\), the fractional Laplacian as
where \(\widehat{u}\equiv {\mathfrak {F}}(u)\) is the Fourier transform of u. It is well known (see [18, 27, 29]) that this operator can be also represented, for suitable functions, as a principal value of the form
where
is a normalizing constant chosen to guarantee that (2.1) is satisfied (see [9, 25, 29]). From (2.2) one can check that
This motivates the introduction of the space
endowed with the natural norm
Then, if \(u\in {\mathcal {L}}^{s}({\mathbb {R}}^{N})\) and \(\phi \in {\mathcal {S}}({\mathbb {R}}^{N})\), using (2.4), we can formally define the duality product \(\langle (-\Delta )^{s}u, \phi \rangle \) in the distributional sense as
We consider the Sobolev space
endowed with the norm
We also consider the Hilbert space \({\mathfrak {D}}^{s,2}({\mathbb {R}}^N)\), which is the completion of \(C^\infty _c({\mathbb {R}}^N)\) w.r.t. the norm
Furthermore, for any open subset \(\Omega \subseteq {\mathbb {R}}^N \) with smooth boundary \(\partial \Omega \), and for any \(p>1\) let \(W^{s, p}(\Omega )\) be the space of measurable functions \(u:\Omega \rightarrow {\mathbb {R}}\) such that the norm
is finite. In addition, denote by \(W^{s, p}_0(\Omega )\) the closure of \(C^\infty _c(\Omega )\) with respect to the norm \(\Vert \cdot \Vert _{W^{s, p}(\Omega )}\,.\) We set
Moreover, we say that \(u\in W^{s,2}_{\text {loc}}(\Omega )\), if for every compact subset \(K\subset \Omega \) we have that \(u\in W^{s,2}(K)\,.\) We also set
where
\({\mathcal {H}}^s_0(\Omega )\), equipped with the norm
is a Hilbert space. If \(\Omega \) is bounded (see, for example, [13]), then there exists a constant \(C=C(\Omega )>~0\) such that
Thus,
Moreover, \(C^\infty _c(\Omega )\) is dense in \({\mathcal {H}}^s_0(\Omega )\,.\)
In the following we will exploit the following well known Sobolev-type embedding Theorem
Theorem 2.1
(See [1, Theorem 7.58], [9, Theorem 6.5], [19, 26]) Let \(0<s<1\) and \(N>2s\). There exists a constant \(S_{N,s}\) such that, for any measurable and compactly supported function \(u:{\mathbb {R}}^{N}\rightarrow {\mathbb {R}}\), we have
where
is the Sobolev critical exponent.
Now we are in position to give the following
Definition 2.2
We say that \(u\in W^{s,2}_{{\text {loc}}}({\mathbb {R}}^N{\setminus }\Gamma )\cap L^{1}({\mathbb {R}}^N)\) is a weak solution to (1.1) if
and
where \(c_{N,s}\) has been defined in (2.3).
For the reader’s convenience, in order to show that Definition 2.2 is well posed, we prove the following
Proposition 2.3
Let \(u\in W^{s,2}_{{\text {loc}}}({\mathbb {R}}^N{\setminus }\Gamma )\cap L^{1}({\mathbb {R}}^N)\). Then, for any \(\varphi \in C^\infty _c(\Omega {\setminus }\Gamma )\),
Proof
Let \(\varphi \in C^\infty _c(\Omega {\setminus }\Gamma )\) and let us denote \(K_{\varphi }= {\text {supp}}(\varphi ) \). Fix now a compact set \( K\subset \Omega {\setminus }\Gamma \) such that \(K_\varphi \subset K\) and use the decomposition
where \(K^c:= {\mathbb {R}}^N {\setminus } K\). Thus,
since
We prove that all the three terms on the right-hand side of (2.7) are finites. In fact
for some positive constant C, since by hypothesis \(u\in W^{s,2}_{{\text {loc}}}({\mathbb {R}}^N{\setminus }\Gamma )\) and \(K\subset \Omega {\setminus }\Gamma \). Therefore, by Hölder inequality, (2.8) follows.
We can write the second term as
We observe that, for all points \((x,y)\in K_\varphi \times K^c\), we have that \(|x-y|\ge \delta >0\), for some positive constant \(\delta =\delta (K,K_\varphi )\). We deduce
with \(C=C(\delta ,K,K_\varphi , \Vert u\Vert _{L^1({\mathbb {R}}^N)}, \Vert \varphi \Vert _{L^{\infty }(K_{\varphi })})\) a positive constant. Here we have used the fact that \(u\in L^1({\mathbb {R}}^N)\) and \(\varphi \in C^\infty (K_{\varphi })\). From (2.9) and (2.10) we obtain
For the third term we argue in the same way as in (2.9), (2.10) and (2.11). Finally, by (2.7) we obtain the thesis. \(\square \)
For future use we point out the following
Lemma 2.4
Let \(u\in W^{s,2}_{{\text {loc}}}({\mathbb {R}}^N{\setminus }\Gamma )\cap L^{1}({\mathbb {R}}^N)\) be a weak solution to (1.1), according to Definition 2.2. Then,
for any \(\varphi \in W^{s,2}_0(\Omega {\setminus }\Gamma )\) with compact support in \(\Omega {\setminus }\Gamma \).
Proof
For any \(\varphi \in W^{s,2}_0(\Omega {\setminus }\Gamma )\) with compact support in \(\Omega {\setminus }\Gamma \), by a convolution argument, we can consider a sequence of functions \(\varphi _n\) with compact support still in \(\Omega {\setminus }\Gamma \) such that
Plugging \(\varphi _n\) as test function in (1.1) and passing to the limit we obtain the thesis. It is crucial here the fact that, by the properties of the convolution, we can assume that the supports of the functions involved remain bounded away from the singular set. \(\square \)
For any given compact subset \(\Gamma \subset \Omega \) we define the relative s-capacity of \(\Gamma \) w.r.t. \(\Omega \) as follows (see, for example, [13]):
Moreover, we define the s-capacity of \(\Gamma \) by
We have the next result.
Lemma 2.5
Let \(\Omega \subset {\mathbb {R}}^N\) be an open bounded subset; let \(\Gamma \subset \Omega \) be a compact subset. Then, there exists a constant \(K>1\) such that
Note that an estimate similar to (2.14) is established in [30]; however, in [30] a slightly different definition of s-capacity is used. Moreover, the relation between the s-capacity and the Haussdorf measure is described also with various examples.
Proof
In view of (2.12) and (2.13), clearly, we have that
Note that, due to (2.13), for any \(\epsilon >0\) there exists \(\phi _\epsilon \in C^\infty _c({\mathbb {R}}^N)\) such that
We can select (see [9]) an open subset \(\Omega '\subset \subset \Omega \) and a function \(\eta _\epsilon \in W^{2, s}({\mathbb {R}}^N)\) such that
Moreover, we can find a constant \(\tilde{C}=\tilde{C}(\Omega ')>0\) such that
Note that thanks to (2.18), we have that \(\eta _\epsilon \in {\mathcal {H}}^s_0(\Omega )\,.\) Using the fact that \(C^\infty _c(\Omega )\) is dense in \({\mathcal {H}}^s_0(\Omega )\), (2.19), and Theorem 2.1, we can infer that
for some positive constant C independent of \(\epsilon \). Letting \(\epsilon \rightarrow 0^+\), we get
This combined with (2.12) yields (2.14). The proof is complete. \(\square \)
We will use the following notations. For a real number \(\lambda \le 0\) we set
which is the reflection trough the hyperplane \(T_\lambda \) and
Also we define
Notation. Generic fixed and numerical constants will be denoted by C (with subscript in some case), and they will be allowed to vary within a single line or formula. By |A| we will denote the Lebesgue measure of a measurable set A.
3 Proof of Theorem 1.1
For \(\lambda <0\) we introduce the following function
where \((u-u_\lambda )^+:=\max \{u-u_\lambda ,0\}\) and \((u-u_\lambda )^-:=\min \{u-u_\lambda ,0\}\). We set
It is not difficult to see that
Lemma 3.1
Under the assumptions of Theorem 1.1 and for \(a<\lambda <0\), we have that
Consequently \( w_\lambda \in {\mathcal {H}}^s_0(\Omega _\lambda \cup R_\lambda (\Omega _\lambda ))\).
Proof
We start by exploiting the fact that the singular set \(\Gamma \) has zero s-capacity. For each \(\varepsilon >0\), let
In view of Lemma 2.5, we have that, for each \(\varepsilon >0\), \({\text {Cap}}_s^{\Gamma _\varepsilon ^\lambda }(R_\lambda (\Gamma ))=0\). Hence, we can find \(\phi _\varepsilon \in C^\infty _c(\Gamma _\varepsilon ^\lambda )\) such that
with \(\phi _\varepsilon \ge 1\) on a neighborhood of \(R_\lambda (\Gamma )\). Via a truncation argument it follows that we can assume \(0\le \phi _\varepsilon \le 1\), \(\phi _\varepsilon \in {\mathcal {H}}^s_0(\Gamma _\varepsilon ^\lambda )\). Let now
and consider
Moreover, we extend \(\varphi _\varepsilon ^\lambda \) by even reflection in \({\mathbb {R}}^N{\setminus }\Sigma _\lambda \), namely \(\varphi _\varepsilon ^\lambda (x)=\varphi _\varepsilon ^\lambda (x_\lambda )\) for every \(x\in {\mathbb {R}}^n{\setminus }\Sigma _\lambda \). In the following, for simplicity, we use the notation \(\varphi _\varepsilon ^\lambda =\varphi _\varepsilon \). Then, we set
It is easy to check that
in the sense of Definition 2.2 . By density arguments (see Lemma 2.4), we can plug \(\varphi \) as test function in Eq. (1.1) fulfilled by u, and in Eq. (3.7) fulfilled by \(u_\lambda \). Arguing in this way and subtracting, we get
where we also used the monotonicity properties of \(f(\cdot ,u)\).
Claim: Now we claim that
To prove this we follow closely the technique in [12] and we argue as follows. We have that
where
Now, we prove that
To check this, we use the decomposition
where \({\mathcal {S}}_\lambda \), \({\mathcal {S}}_\lambda ^c\), \({\mathcal {D}}_\lambda \) and \({\mathcal {D}}_\lambda ^c\) have been introduced in (3.2). By construction, it follows that
We have that
Indeed, note that, if \(x\in {\mathcal {S}}^c_\lambda \) and \(y\in {\mathcal {S}}_\lambda \), then \({\mathcal {G}}(x,y)\ge 0\); moreover, \({\mathcal {G}}(x,y)=-{\mathcal {G}}(x,y_\lambda )\). Also, we have that \(|x-y|\le |x-y_\lambda |\) for all \((x,y)\in {\mathcal {S}}_\lambda ^c \times {\mathcal {S}}_\lambda \). Therefore, using also (3.3), we have
which shows (3.12). Similarly, one can prove that
and
Collecting the estimates above we obtain (3.11) that actually proves (3.9) and the claim.
By (3.9) it follows now that (3.8) provides
that we rewrite as
Observe now that, by a symmetry argument, we have
On the other hand, using the Young inequality we have
In the following computations we set \(\varepsilon =\frac{1}{8} c_{N,s}\) and, taking into account (3.14), by (3.15) and (3.16), we arrive at
In the final estimate we exploited the properties of the cutoff function provided by (3.6) and the fact that \(0\le w_\lambda \le u\) in \(\Omega _\lambda \) (together with a symmetry argument).
Then, since \(\varphi _\varepsilon \rightarrow 1\) in \({\mathbb {R}}^N\) as \(\varepsilon \rightarrow 0^+\), the inequality (3.4) follows by Fatou Lemma letting \(\varepsilon \rightarrow 0^+\) in (3.17).
To deduce that \( w_\lambda \in {\mathcal {H}}^s_0(\Omega _\lambda \cup R_\lambda (\Omega _\lambda ))\) just note that \(w_\lambda \) is bounded and then apply standard arguments, see [9]. \(\square \)
Proof of Theorem 1.1
We start the moving plane procedure by showing that, recalling (2.24), we can take \(a<\lambda <0\), with \(|\lambda -a|\) small, in such a way that \(u\le u_\lambda \) in \(\Omega _\lambda {\setminus } R_\lambda (\Gamma )\). In fact using \(\varphi \,:=\, w_\lambda \varphi _\varepsilon ^2\) in Eq. (1.1) fulfilled by u and in Eq. (3.7) fulfilled by \(u_\lambda \), subtracting we get
and then, as in (3.13) (see also (3.9)), we have
Using that \(\varphi _\varepsilon ^2\le 1\) in all \({\mathbb {R}}^N\) and that \(w\in L^{\infty }({\mathbb {R}}^N)\), it follows
and \(C=C(\Vert u\Vert _{L^\infty (\Omega _\lambda )})\) is a positive constant. Therefore, by Lemma 3.1, (3.5) and (3.6) we deduce
where C is a positive constant not depending on \(\varepsilon \). Letting \(\varepsilon \) tend to zero, the l.h.s of (3.18) by weak convergence goes to
By (\(A_f^1\)) and Lemma 3.1, the r.h.s of (3.18) goes to
Hence, (3.18) becomes
Using (\(A_f^1\)) and Hölder inequality, it follows
where the last inequality follows from Theorem 2.1. Recalling (2.24), for \(|\lambda -a|\) small, it follows that
A contradiction occurs by (3.20) unless
that is \(u\le u_\lambda \) in \(\Omega _\lambda \).
Let us now set
and
that is well defined since we showed that \(\Lambda _0\) is not empty. To prove our result we have to show that \(\lambda _0 = 0\).
To prove this we assume that \(\lambda _0<0\) and we reach a contradiction by proving that \(u\le u_{\lambda _0+\tau }\) in \(\Omega _{\lambda _0+\tau }{\setminus } R_{\lambda _0+\tau }(\Gamma )\) for any \(0<\tau <\bar{\tau }\) for some small \(\bar{\tau }>0\). By continuity of u in \(\bar{\Omega }{\setminus } \Gamma \), we know that \(u\le u_{\lambda _0}\) in \(\Omega _{\lambda _0}{\setminus } R_{\lambda _0}(\Gamma )\). Actually it follows that \(u< u_{\lambda _0}\) in \(\Omega _{\lambda _0}{\setminus } R_{\lambda _0}(\Gamma )\). To deduce this, just write down the equation fulfilled by \(u- u_{\lambda _0}\) and exploit Proposition 3.6 in [17].
Therefore, given a compact set \(K\subset \Omega _{\lambda _0}{\setminus } \overline{R_{\lambda _0}(\Gamma )}\), by a uniform continuity argument, we can ensure that \(u< u_{\lambda _0+\tau }\) in K for any \(0<\tau <\bar{\tau }\) for \(\bar{\tau }>0\) small. Note that to do this we implicitly assume, with no loss of generality, that \(R_{\lambda _0+\tau }(\Gamma )\) remains bounded away from K. Arguing as in Lemma 3.1 we consider
with the same construction and we set
In view of Lemma 3.1, we can choose \(\varphi \) as test function arguing exactly as in the proof of Lemma 3.1 and again we arrive at the first inequality in (3.17), namely
By construction, see (3.6), it follows that
Therefore, arguing as above, we pass to the limit as \(\varepsilon \rightarrow 0\) and, recalling Lemma 3.1, we deduce that
By the Sobolev inequality, see Theorem 2.1, we deduce that
where the \(C(\cdot )\) involves now the Sobolev constant. For K large and \(\bar{\tau }\) small, we may assume that
so that, by (3.21), we deduce that
This proves that \(u\le u_{\lambda _0+\tau }\) in \(\Omega _{\lambda _0+\tau }{\setminus } R_{\lambda _0+\tau }(\Gamma )\) for any \(0<\tau <\bar{\tau }\) and for some small \(\bar{\tau }>0\). Such a contradiction shows that
Since the moving plane procedure can be performed in the same way but in the opposite direction, then this proves the desired symmetry result. The fact that the solution is increasing in the \(x_1\)-direction in \(\{x_1<0\}\) is implicit in the moving plane procedure. If \(\Omega \) is a ball and u has only a nonremovable singularity at the origin, then the solution is radial and radially decreasing about the center of the ball. This follows applying the moving plane procedure in any direction \(\nu \in {\mathbb {S}}^1\) of \({\mathbb {R}}^N\). \(\square \)
4 Proof of Theorem 1.2
We start by proving the following
Lemma 4.1
Under the assumptions of Theorem 1.2, for \(\lambda <0\), we have that
where \(C=C(f, s, N, \Vert u\Vert _{L^{2^*_s}({\mathbb {R}}^N{\setminus } B_{R_0})}, \Vert u\Vert _{L^\infty (\Sigma _\lambda \cap B_{R_0})})\) is a positive constant.
Proof
We start by exploiting the fact that the singular set \(\Gamma \) has zero s-capacity. For each \(\varepsilon >0\), let
Arguing as in the case of a bounded domain, thanks to Lemma 2.5, we have that, for each \(\varepsilon >0\), \({\text {Cap}}_s^{\Gamma _\varepsilon ^\lambda }(R_\lambda (\Gamma ))=0\). Therefore, there exists \(\phi _\varepsilon \in C^\infty _c(\Gamma _\varepsilon ^\lambda )\) such that
with \(\phi _\varepsilon \ge 1\) on a neighborhood of \(R_\lambda (\Gamma )\). Via a truncation argument it follows that we can assume \(0\le \phi _\varepsilon \le 1\), \(\phi _\varepsilon \in H^s_0(\Gamma _\varepsilon ^\lambda )\). Let \(\varphi _\varepsilon ^\lambda (x)\) be defined in \(\Sigma _\lambda \) as in (3.6). Then, by even reflection, we define \(\varphi _\varepsilon ^\lambda (x)\) in all \({{\mathbb {R}}}^N\) putting \(\varphi _\varepsilon ^\lambda (x)=\varphi _\varepsilon ^\lambda (x_\lambda )\) for every \(x\in {\mathbb {R}}^n{\setminus }\Sigma _\lambda \). Let \(\varphi _{1,0}\in C^{\infty }({\mathbb {R}}^N)\) be a standard cutoff function such that \(\varphi _{1,0}=1\) in \(B_1(0)\) and \(\varphi _{1,0}=0\) outside \(B_{2}(0)\) and even w.r.t the hyperplane \(T_0\), i.e., \(\varphi _{1,0}(x)=\varphi _{1,0}(x_0)\) for every \(x\in {\mathbb {R}}^n{\setminus }\Sigma _0\). Then, for a fixed point \(x_C\in T_\lambda \), let us set \(\varphi _{R,x_c}=\varphi _{1,0}((x-x_C)/R)\). Recalling (3.1) we set
We point out that \(u_\lambda \) (see (2.23)) solves
in the sense of Definition 2.2. By density arguments (see Lemma 2.4), we can plug \(\varphi \) as test function in Eq. (1.2) fulfilled by u and in equation (4.3) fulfilled by \(u_\lambda \). Subtracting, we get
Arguing as in the proof of Lemma 3.1, following verbatim the computations from Eq. (3.9) to equation (3.13), we obtain
We rewrite (4.5) as
Recalling (3.15) we have
On the other hand, using the Young inequality we have
Now we set \(\delta =\frac{1}{8} c_{N,s}\) and, taking into account (4.6), by (4.7) and (4.8) we obtain
where C is a positive constant depending on s, N. Let us start by evaluating the term \(I_1\). First of all we obtain
where we also used that \(\varphi ^2_R\le 1\), \(\varphi ^2_\varepsilon \le 1\) in a \({\mathbb {R}}^N\). In the following we exploit some standard arguments, see, for example, [10]. In our case such an application would be more easy in the case of globally bounded solutions. Since we deal with the more general case of locally bounded solutions, the computations are more involved.
To estimate the term \(I_{11}\), we define the following sets:
Therefore,
Define \(\sigma _0=s\) and fix \(\sigma _1\in (0,s)\) and \(\sigma _2\in (s,1)\). Let us write now, for \(k=0,1,2,\)
By Hölder inequality, for \(k=\{0,1,2\}\), we have
The first integral on the r.h.s of (4.13), by the change of variable \(\hat{x}=(x-x_C)/R\) can be estimated as
For the second integral on the r.h.s of (4.13) we proceed decomposing it on the three sets (4.11).
Let \(k=0\). When \((x,y)\in A_{0}(x_C)\) we have that \(|x-y|\ge |y-x_C|-|x-x_C|\ge |y-x_C|/2\) and therefore
with \(C=C(N)\) a positive constant and where we used the fact that \(\sigma _0=s\).
Let \(k=1\). Recalling that \(\sigma _1\in (0,s)\), we obtain
where in the last line we used the change of variable \(\hat{x}=x-y\) and where \(C=C(s,\sigma _1,N)\) is a positive constant.
Let \(k=2\). Recalling that \(\sigma _2\in (s,1)\), we deduce
where \(C=C(s,\sigma _2,N)\) is a positive constant.
Collecting (4.15), (4.16) and (4.17) we have that
From (4.13), using (4.14) and (4.18) it follows
where C is a positive constant not depending on R. Finally from (4.12), we obtain
with \(R_0\) given in the statement of Theorem 1.2 and where \(C_{11}\) is a positive constant that does not depend on R (and on \(\varepsilon \)). We point out that, in the last line of (4.20) we used the fact that \(w_\lambda (x)\le u(x)\), \(u\in L^{2^*_s}({\mathbb {R}}^N{\setminus } B_{R_0})\) and that, by (3.1), \(w_\lambda \in L^{\infty }(B_{R_0})\). To estimate the term \(I_{12}\) in (4.10), we fix a radius \(\hat{R}>R_0\) such that \(\overline{B_{R_0} \cup R_\lambda (B_{R_0})} \subset B_{\hat{R}}\). Therefore, using that (see (3.6)) \(\varphi _\varepsilon ^\lambda (x)=1\) in \({\mathbb {R}}^N{\setminus } B_{\hat{R}}\)
By Definition (3.1) we have that \(w_\lambda \in L^{\infty }(B_{\hat{R}})\). Thus, using (4.2) we obtain
where, \(A_{\hat{R}}:=R_\lambda (B_{\hat{R}})\) and \(C=C(\Vert u\Vert _{L^{\infty }(A_{\hat{R}})})\) is a positive constant. Similarly we also get
For the last term of (4.21) we argue splitting it in two terms:
For the first term, as we did in (4.22), we have
with \(C=C(\Vert u\Vert _{L^{\infty }(A_{2\hat{R}})})\). For the second term we use Hölder inequality deducing
with \(C=C(s, N, \hat{R},\Vert u\Vert _{L^{2^*_s}({\mathbb {R}}^N{\setminus } B_{2\hat{R}})}, \Vert u\Vert _{L^{\infty }(A_{2\hat{R}})})\). Since for all \((x,y)\in B_{\hat{R}} \times {\mathbb {R}}^N{\setminus } B_{2\hat{R}}\), it follows that \(|x-y|\ge \delta >0\), from (4.25) we infer that
and \(C=C(s, N, \hat{R},\Vert u\Vert _{L^{2^*_s}({\mathbb {R}}^N{\setminus } B_{2\hat{R}})}, \Vert u\Vert _{L^{\infty }(A_{2\hat{R}})})\). Using (4.22), (4.23) and (4.26), from (4.21) we deduce
Finally from (4.10), collecting (4.20) and (4.27) it follows
for some positive constant \(C_1\).
To estimate \(I_2\) in (4.9) we use the mean value theorem and (\(A_f^2\)). In fact
where \(C_2(f, \Vert u\Vert _{L^{2^*_s}({\mathbb {R}}^N{\setminus } B_{R_0})}, \Vert u\Vert _{L^\infty (\Sigma _\lambda \cap B_{R_0})})\). Using (4.28) and (4.29) and redefining the constants, from (4.9) we have
The thesis follows now by Fatou Lemma as (first) \(\varepsilon \) tends to zero and (then) R tends to infinity. \(\square \)
Proof of Theorem 1.2
We start the moving plane procedure by showing that for \(\lambda <0\) and \(|\lambda |\) large, we obtain that \(u\le u_\lambda \) in \(\Sigma _\lambda {\setminus } R_\lambda (\Gamma )\). In fact using \(\varphi \,:=\, w_\lambda \varphi _\varepsilon ^2\varphi _{R,x_c}^2\) in Eq. (1.2) fulfilled by u and in Eq. (4.3) fulfilled by \(u_\lambda \), subtracting we get (see Eq. (4.4))
and then, as in (4.5), we have
Using that \(\varphi _\varepsilon ^2\varphi _{R,x_c}^2\le 1\) in all \({\mathbb {R}}^N\), it follows
and therefore, by Lemma 4.1, (4.9), (4.10) and (4.20)
with C is a positive constant not depending on \(\varepsilon \) and R. Letting first \(\varepsilon \) to zero and then R to infinity, using Lemma 4.1 and (4.31), the l.h.s of (4.30) by weak convergence goes to
By (\(A_f^2\)) and Lemma 4.1, the r.h.s of (4.30), by the dominate convergence Theorem goes to
Hence, (4.30) becomes
Using (\(A_f^2\)) and Hölder inequality, it follows
where the last inequality follows from Theorem 2.1. Recalling that \(u\in L^{2^*_s}({\mathbb {R}}^N{\setminus } B_{R_0})\), with \(\Gamma \subset \{x_1=0 \}\cap B_{R_0}\) we deduce that we can take \(\lambda <0\), with \(|\lambda |\) large, in such a way that
A contradiction occurs by (4.32) unless
that is \(u\le u_\lambda \) in \(\Sigma _\lambda \).
Let us now set
and
that is well defined since we showed that \(\Lambda _0\) is not empty. To prove our result we have to show that \(\lambda _0 = 0\). To prove this we assume that \(\lambda _0<0\) and we reach a contradiction by proving that \(u\le u_{\lambda _0+\tau }\) in \(\Sigma _{\lambda _0+\tau }{\setminus } R_{\lambda _0+\tau }(\Gamma )\) for any \(0<\tau <\bar{\tau }\) for some small \(\bar{\tau }>0\). By continuity of u in \({\mathbb {R}}^N{\setminus } \Gamma \), we know that \(u\le u_{\lambda _0}\) in \(\Sigma _{\lambda _0}{\setminus } R_{\lambda _0}(\Gamma )\). By the strong maximum principle ([17, Proposition 3.6]) we deduce that \(u< u_{\lambda _0}\) in \(\Sigma _{\lambda _0}{\setminus } R_{\lambda _0}(\Gamma )\). Here we use that a symmetry position before the limiting position (namely \(u= u_{\lambda _0}\) in \(\Sigma _{\lambda _0}{\setminus } R_{\lambda _0}(\Gamma )\)) is not possible, if \(\lambda _0<0\), since in this case u should be singular on \(R_{\lambda _0}(\Gamma )\) . For \(\delta >0\) that will be chosen small later on, we consider a compact set \(K_\delta \subset \Sigma _{\lambda _0}{\setminus } R_{\lambda _0}(\Gamma )\) such that
By uniform continuity, we can take \(\bar{\tau }\) small such that \(u< u_{\lambda _0+\tau }\) in \( K_\delta \) for any \(0<\tau <\bar{\tau }\). Now we repeat verbatim the arguments used at the beginning of this proof, using the test function \(\varphi \,:=\, w_{\lambda _0+\tau }\varphi _\varepsilon ^2\varphi _{R,x_c}^2\) in Eq. (3.7) fulfilled by u and in Eq. (4.3) fulfilled by \(u_\lambda \). Taking the limits, as in (4.32), we have
Now we chose \(\delta \) small in such a way that
obtaining the desired contradiction by (4.33) and showing that \(\lambda _0 = 0\). The symmetry of the solution follows now performing the moving plane method in the opposite direction. The monotonicity of the solution is implicit in the technique.
If u has only a nonremovable singularity at the origin, then the solution is radial and radially decreasing about the origin. This follows applying the moving plane procedure in any direction \(\nu \in {\mathbb {S}}^1\) of \({\mathbb {R}}^N\). \(\square \)
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The authors are partially supported by the Gnampa Project 2016 ‘Proprietà qualitative di equazioni ellittiche e paraboliche non lineari’
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Montoro, L., Punzo, F. & Sciunzi, B. Qualitative properties of singular solutions to nonlocal problems. Annali di Matematica 197, 941–964 (2018). https://doi.org/10.1007/s10231-017-0710-z
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DOI: https://doi.org/10.1007/s10231-017-0710-z