Abstract
We consider the following fractional Hénon type equation with critical growth:
where K(|y|) is a bounded function defined in [0, 1], \(B_1(0)\) is the unit ball in \({\mathbb {R}}^{N}\), \(N\ge 3\) for \(\frac{3}{4} \le s<1\) and \(3\le N < 2s -1 +\frac{2}{3-4s}\) for \(\frac{11-\sqrt{41}}{8}< s<\frac{3}{4}\). We show that if \(K(1)>0\) and \(K'(1)>0\), then equation (0.1) has infinitely many non-radial positive solutions, whose energy can be made arbitrarily large. The most ingredients of the paper are using the Green representation and estimating the Green function and its regular part very carefully. For this purposes, some more extra ideas and techniques are needed. We believe that our method and techniques can be applied to other related problems.
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1 Introduction
In this paper, we are concerned with the following fractional Hénon type equation with critical growth:
where K(|y|) is a bounded function defined in [0, 1], \(B_1(0)\) is the unit ball in \({\mathbb {R}}^{N}\), \(N\ge 3\) for \(\frac{3}{4} \le s<1\) and \(3\le N < 2s -1 +\frac{2}{3-4s}\) for \(\frac{11-\sqrt{41}}{8}< s<\frac{3}{4}\). \((-\Delta )^{s}\) is the so called fractional operator defined as:
where P.V. is the principal value and \(C(N,s) =\pi ^{-(2s+\frac{N}{2})}\frac{\Gamma (\frac{N}{2}+s)}{\Gamma (-s)}\). The fractional Laplacian operator appears in many areas including astrophysics, mathematical finances and so on, and it can be regarded as the infinitesimal generator of a stable Levy process (see [1]). For more results related to fractional operators, we refer readers to [3,4,5,6, 11, 13, 19, 20, 23] and the references therein.
The classical Hénon equation states that
where \(\alpha > 0\), \(q>0\) are positive constants. This equation was first introduced by Hénon in the study of astrophysics (see [10]). It has attracted lots of interests in recent years. In the subcritical case, that is \(q<\frac{N+2}{N-2}\), the existence of the solution for problem (1.2) can be proved easily by variational methods. For the critical case, that is \(q=\frac{N+2}{N-2}\), the loss of compactness of embedding from \(H^{1}_{0}(B_{1}(0))\) to \(L^{\frac{2N }{N-2}}(B_{1}(0))\) makes the problem (1.2) very difficult to study. Ni [14] observed the influence of the non-autonomous term \(|y|^\alpha \) and proved that it possesses a positive radial solution when \(q \in (1, \frac{N+2+2\alpha }{N-2})\).
It is natural to ask whether (1.2) has a non-radial solution. When \(N=2\), Smets-Su-Willem [18] showed that the mountain pass solution is non-radial when \(\alpha \) is large. When \(N \ge 3\) and \(q = \frac{N+2}{N-2}-\epsilon \) with \(\epsilon \) is small (near critical), Cao-Peng [7] proved that the mountain pass solution is non-radial and it blows up as \(\epsilon \rightarrow 0\). Using a variational method, Serra [17] proved that (1.2) has a non-radial solution when \(N\ge 4\), \(q=\frac{N+2}{N-2}\) and \(\alpha \) is large. While Wei-Yan [21] proved there exists infinitely many non-radial solutions for \(N\ge 4\), \(q=\frac{N+2}{N-2}\) and any \(\alpha > 0\). And this result was later extended to the polyharmonic case by Guo and Li [8].
Before the statement of the main result, we introduce some notations.
Let \( H_{0}^s(\Omega )=\{ u\in H^s({\mathbb {R}}^{N}): u =0 \hbox { in } \Omega ^c \}\) with the norm:
We fix a positive integer \(k\ge k_0\), where \(k_0\) is large enough, which will be determined later. Set \(\mu =k^{\frac{N-2s+1}{N-2s}}\) be the scaling parameter, where \( N\ge 3\) when \(\frac{3}{4}\le s <1\) and \( 3\le N < 2s -1 +\frac{2}{3-4s}\) when \(\frac{11-\sqrt{41}}{8}< s<\frac{3}{4}\).
Let \(2^{*}_s = \frac{2N}{N-2s}\). By the transformation \(u(y)\rightarrow \mu ^{-\frac{N-2s}{2}}u(\frac{y}{\mu })\), (1.1) becomes to be
In the following, we just need to consider (1.3) instead of (1.1).
It is well known that the functions
where \(\gamma =\frac{\Gamma (\frac{N+2s}{2})}{\Gamma (\frac{N-2s}{2})} \), are the only solutions (usually called bubbles) to the following problem (see [12]):
Noting that when \(y\in B_{1}^{c}(0)\), \(U_{x,\Lambda }(y)\) is not zero, we define \(PU_{x,\Lambda }\) as the projection of \(U_{x,\Lambda }\), that is the solution of the following problem:
Let \(y=(y',y'')\), \(y'\in {\mathbb {R}}^{2}\), \(y''\in {\mathbb {R}}^{N-2}\). Define
Let \( x_j=( r\cos \frac{2(j-1)\pi }{k},r\sin \frac{2(j-1)\pi }{k} ,0 ),\hbox { }j=1,...,k,\) where 0 is the zero vector in \({\mathbb {R}}^{N-2}\), \(r\in [\mu \big (1-\frac{r_0}{k}\big ), \mu \big (1-\frac{r_1}{k}\big ) ],\hbox { for some constants } r_1>r_0>0,\) and \(L_0\le \Lambda \le L_1,\) for some constants \(L_1>L_0>0\). Set
The main result of the present paper is the following:
Theorem 1.1
Suppose that \(N\ge 3\) for \(\frac{3}{4} \le s<1\) and \(3\le N < 2s -1 +\frac{2}{3-4s}\) for \(\frac{11-\sqrt{41}}{8}< s<\frac{3}{4}.\) If K(r) is a bounded function defined in [0, 1] and statisfies \(K(1)>0\) and \(K'(1)>0\), then there is an integer \(k_0>0\), such that for any integer \(k\ge k_0\), (1.3) has a solution \(u_k\) of the form
where \(\omega _k\in H_r\cap H^s_0\big (B_{\mu }(0)\big )\), and as \(k\rightarrow +\infty \), \(||\omega _{k}||_{L^{\infty } }\rightarrow 0\),\( L_0\le \Lambda _k \le L_1\), and \(r_k\in \big [ \mu (1-\frac{r_0}{k}),\mu (1-\frac{r_1}{k}) \big ]\). As a consequence, (1.1) has infinitely many non-radial solutions.
Without loss of generality, in the following, we assume that \(K(1) = 1\).
The proof of Theorem 1.1 is mainly dependent on the finite-dimensional reduction method. The main idea of the reduction argument can be found in [2, 16, 21, 22]. Roughly speaking, to carry out this reduction argument, the first step is to construct a reasonably approximation solution, so that the problem can be reduced to a finite dimensional problem. The second step is to solve the corresponding finite dimensional problem to obtain a true solution. To fulfill the second step, it is essential to obtain a good estimate for the error term in the first step. However, when one consider more complicated problems, both steps must be modified. For example, in [22], to deal with the large number of bubbles in the solution, the reduction procedure is carried out in a weighted space instead of the standard Sobolev space. Our main idea is to place a large number of bubble inside \( B_{\mu }(0)\). Then the scaling parameter will be determined by the number of bubbles. We put many bubbles along a \(k-\)polygon inside the domain \( B_{\mu }(0)\) but near the boundary. Different from [21], the non-local properties of the equation make the problem getting more complicated. In order to decide the location of the bubble points, the most ingredients of the paper are using the Green representation and estimating the Green function and its regular part very carefully. Some more extra ideas and techniques are needed. We believe that our method and techniques can be applied to other related problems.
The paper is organized as follows. In Sect. 2, we perform a finite-dimensional reduction. The proof of Theorem 1.1 will be given in Sect. 3. Energy expansion and some essential estimates are attached in Appendices.
2 Finite-dimensional reduction
In this section, we perform a finite–dimensional reduction. Let
and
where \(\tau = \frac{N-2s}{N-2s+1}\), \(N\ge 3\) for \(\frac{3}{4} \le s<1\) and \(3\le N < 2s -1 +\frac{2}{3-4s} \) for \(\frac{11-\sqrt{41}}{8}< s<\frac{3}{4}\). For this choice of \(\tau \), we find that
Let
We consider the following problem:
for some numbers \(c_i\) where \(\langle u,v \rangle = \displaystyle \int _{B_{\mu }(0)}u v \).
Lemma 2.1
Assume that \(\phi _k\) solves (2.3) for \(h =h_k,\) if \(||h||_{**}\) goes to zero as k goes to infinity, so does \(||\phi _k||_*\).
Proof
We argue by contradiction. Suppose that there are \(k \rightarrow +\infty \), \(h=h_k\), \(\Lambda _k \in [L_1,L_2 ]\), \(r_k \in [\mu (1-\frac{r_0}{k}), \mu (1-\frac{r_1}{k})] \), and \(\phi _k\) solve (2.3) for \(h= h_k\), \( \Lambda = \Lambda _k\) and \(r = r_k\) with \(||h_k||_{**} \rightarrow 0\), and \(||\phi _k||_{*}\ge c'>0 \). We may assume that \(||\phi _k||_{*}=1\). For simplify, we drop the subscript k. By Green representation, we rewrite (2.3) as
Using Lemma C.3, we have
It follows from Lemma C.2 that
and
Next, we estimate \(c_l\), \(l=1,2\). Multiplying (2.3) by \(Z_{1,l}\) and integrating, we see that \(c_{t}\) satisfies
It follows from Lemma C.1 that
On the other hand, using Lemma A.1 and Lemma C.3, we can prove
A direct computation leads to
where \({\bar{c}} >0\) is a constant. Thus we obtain from (2.8) that
So
Since \(||\phi ||_*=1\), we obtain from (2.11) that there exists \(R>0\) such that
for some i. However, \({\bar{\phi }}=\phi (y-x_i)\) converges uniformly in any compact set to a solution u of
for some \(\beta \in [L_1,L_2]\), and u is perpendicular to the kernel of (2.13). Hence, \(u=0\). This is a contradiction to (2.12). \(\square \)
From Lemma 2.1, using the same arguments as in the proof of Proposition 4.1 in [15], we can prove the following result.
Proposition 2.2
There exists \(k_0 >0\) and a constant \(C>0\), independent of k, such that for all \(k\ge k_0\) and all \(h\in L^{\infty }({\mathbb {R}}^{N})\), problem (2.3) has a unique solution \(\phi \equiv L_k(h)\). Moreover
Now, we consider the following problem:
In the rest of this section, we are devoted to the proof of the following proposition by the contraction mapping theorem.
Proposition 2.3
If \(N\ge 3\) for \(\frac{3}{4} \le s<1\) and \(3\le N < 2s -1 +\frac{2}{3-4s} \) for \(\frac{11-\sqrt{41}}{8}< s<\frac{3}{4}\), then there is an integer \(k_0>0\), such that for each \(k\ge k_0\), \(L_0\le \Lambda \le L_1\) and \(r\in [\mu (1-\frac{r_0}{k}),\mu (1-\frac{r_1}{k})]\), (2.15) has a unique solution \(\phi =\phi (r,\Lambda )\), satisfying
where \(\sigma >0\) is a small constant and \(\mu =k^{\frac{N-2s+1}{N-2s}}\).
We rewrite (2.15) as
where
and
In order to use the contraction mapping theorem to prove that (2.16) is uniquely solvable in the set where \(||\phi ||_*\) is small, we need to estimate \(N(\phi )\) and \(l_k\).
Lemma 2.4
If \(N\ge 3\) and \(\frac{11-\sqrt{41}}{8}<s<1\), then
Proof
If \(2^*_s-1\le 2\), we have
So
If \(2^*_s-1 \ge 2\), we have
Thus,
\(\square \)
Next, we estimate \(l_k\).
Lemma 2.5
Assume that \(r\in [\mu (1-\frac{r_0}{k}),\mu (1-\frac{r_1}{k})]\). If \(N\ge 3\) for \(\frac{3}{4} \le s<1\) and \(3\le N < 2s -1 +\frac{2}{3-4s} \) for \(\frac{11-\sqrt{41}}{8}< s<\frac{3}{4}\), then
Proof
Define
We have
By the symmetry, we assume that \(y\in \Omega _1\). Then for \(\forall y\in \Omega _1\), \(j = 2, ...,k\), we have
For the estimate of \(J_0\), we have
On the one hand, since \(2s-\tau >\frac{1}{2}\), we have
On the other hand, we have
and
Thus, we have
Now we estimate \(J_1\). We have
Similar to the estimate of \(J_{00}\), we obtain
For the estimate of \(J_{10}\), we have
Let \(r_3=\min (r_0,1),\) if \( |y-x_1|\ge \frac{r_3\mu }{8k},\) we get
And if \(|y-x_1|\le \frac{r_3\mu }{8k} \), using Lemma A.1, we have
So,
Similarly, we can prove
Thus,
So
Now we estimate \(J_2\). It is easy to check that
If \( |y-x_1|\ge \frac{r_0\mu }{2k} \), we have
And if \( |y-x_1|\le \frac{r_0\mu }{2k} \), we have
So,
Combining (2.26), (2.27) and (2.28), we obtain
Finally combining (2.18), (2.25) and (2.29), it holds
\(\square \)
Now, we are ready to prove proposition 2.3.
.
Proof of Proposition 2.3
Recall that \(\mu = k^{\frac{N-2s+1}{N-2s}}\), \(N\ge 3\) for \(\frac{3}{4} \le s<1\) and \(3\le N < 2s -1 +\frac{2}{3-4s} \) for \(\frac{11-\sqrt{41}}{8}< s<\frac{3}{4}\).
Let
Then (2.16) is equivalent to
where \(L_k\) is defined in Proposition 2.2. We will prove that A is a contraction map from E to E. First, we have
On the other hand,
If \(2^{*}_s-2 \le 1\), then
As a result, we obtain
Similar to the arguments for \(||N(\phi )||_*\) , we have
Thus, we obtain
As a result, A is a contraction map.
If \(2^{*}_s-2 \ge 1\), then \( |N'(t)|\le C|t|^{2^{*}_s-2} + CW_{r,\Lambda }^{2^{*}_s-3}|t|. \) Hence,
Thus A is a contraction map.
By the contraction mapping theorem, there exists a unique \(\phi \in E\), such that \( \phi =A(\phi ).\) Moreover, it follows from Proposition 2.2 that
which leads to
The estimate of \(c_t\) follows from (2.14). \(\square \)
3 Proof of theorem 1.1
Let
where \(r=|x_1|\), \(d=1-\frac{r}{\mu }\), \(\phi \) is the function obtained in Proposition 2.3 and
Let \({\bar{x}}_j=\frac{1}{\mu }x_j\), G(x, y) be the Green function of \((-\Delta )^{s}\) in \(B_{1}(0)\) with homogenous Dirichlet boundary condition and H(x, y) be the part of the Green function.
Proposition 3.1
If \(N\ge 3\) for \(\frac{3}{4} \le s<1\) and \(3\le N < 2s -1 +\frac{2}{3-4s} \) for \(\frac{11-\sqrt{41}}{8}< s<\frac{3}{4}\), then
where A, \(A_1\), \(A_2\), \(A_3\), \(B_1\) and \(B_2\) are positive constants, and \(\sigma >0\) is a small constant.
Proof
Since
there is \(t\in (0,1)\) such that
However,
By Lemma C.1, for \(N\ge 3\),
Thus, we obtain
On the other hand,
Noting that for \(y\in \Omega _1\) and \(N\ge 3\)
Thus, we have
which leads to
So, we have proved
Thus,
And (3.1) follows from Proposition B.1. \(\square \)
Proposition 3.2
If \(N\ge 3\) for \(\frac{3}{4} \le s<1\) and \(3\le N < 2s -1 +\frac{2}{3-4s} \) for \(\frac{11-\sqrt{41}}{8}< s<\frac{3}{4}\), then we have
and
where \(A_1\), \(A_2\), \(A_3\), \(B_1\) and \(B_2\) are the same constants as in Proposition 3.1, and \(\sigma > 0\) is a small constant.
Proof
We estimate \(\frac{\partial F(d,\Lambda )}{\partial \Lambda }\) first. We have
Noting that
we have
On the other hand,
If \(2^{*}_s-1 \le 2 \), we have
If \(2^{*}_s-1 \ge 2 \), we have
Thus, we have
Noting that \(\phi \in E\), so we have
and using Lemma A.1, if \(2^{*}_s-2\le 1 \), we have
If \( 2^{*}_s-2\ge 1 ,\) we have
On the other hand,
where \(r_3=\min (r_0,1)\). Thus, we have proved
and (3.2) follows from Proposition B.2.
Finally using Proposition B.2, we can estimate \(\frac{\partial F(d,\Lambda )}{\partial d} \) in a similar way. \(\square \)
Now we are ready to prove Theorem 1.1.
Proof of Theorem 1.1
Note that \(d =1 -\frac{r}{\mu }\) and \(\mu = k^{\frac{N-2s+1}{N-2s}}\). Define \(D =dk\). Then from (3.2) and (3.3), \( \frac{\partial F(d,\Lambda )}{\partial \Lambda } =0 \) and \( \frac{\partial F(d,\Lambda )}{\partial d} =0 \) are equivalent to
and
respectively.
Let
and
Since \(\displaystyle \lim _{D\rightarrow 0}f_3(D) =-\infty \) and \(\displaystyle \lim _{D\rightarrow +\infty }f_3(D) > 0\), there is a positive constant \( D_0\), such that \( f_3(D_0) =0\). So for any \(\Lambda >0\), \(f_1(D_0,\Lambda ) =0\).
On the other hand, when \( \Lambda _0\! =\! \big (\frac{\frac{A_1(N-2s)}{D_0^{N-2s+1}} +A_3(N-2s)\sum _{i=2}^{+\infty }\frac{1}{((i-1)\pi )^{N}}\big ( \frac{D_0^{2}}{((i-1)\pi )^{2}} +1 \big )^{\frac{-N}{2}}D_0^{2s-1} }{A_2}\big )^{\frac{1}{N-2s}}\), \(f_2(D_0,\Lambda _0) = 0\). Moreover, it is easy to check that
and
Thus the linear operator of \(f_1=0\) and \(f_2=0\) at \((D_0,\Lambda _0)\) is invertible. As a result, (3.4) and (3.5) have a solution near \(( D_0,\Lambda _0)\). \(\square \)
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Appendices
Appendix A. The estimate of the projection
In both appendices, we always assume that
where 0 is the zero vector in \({\mathbb {R}}^{N-2}\), and \(r\in [ \mu (1-\frac{r_0}{k}), \mu (1-\frac{r_1}{k}) ]\). Recall that \( {\bar{x}}_j=\frac{1}{\mu }x_j. \) G(x, y) be the Green function of \((-\Delta )^{s}\) in \(B_{1}(0)\) with homogenous Dirichlet boundary condition. H(x, y) be the part of the Green function. \(PU_{x,\Lambda }\) is the solution of (1.4) and \(r_3 =\min ( r_0,1)\).
For \(l=1,..,N\), we denote \(\partial _l PU_{x,\Lambda }(y) = \frac{\partial PU_{x,\Lambda } (y) }{\partial x_l}\), \(\partial _l U_{x,\Lambda }(y) = \frac{\partial U_{x,\Lambda } (y) }{\partial x_l} \), and \( \partial _l H(x,y) = \frac{\partial H }{\partial x_l}(x,y)\). For \(l=N+1\), we set \(\partial _l PU_{x,\Lambda }(y) = \frac{\partial PU_{x,\Lambda } (y) }{\partial \Lambda }\), and \(\partial _l U_{x,\Lambda }(y) = \frac{\partial U_{x,\Lambda } (y) }{\partial \Lambda } \).
Lemma A.1
Assume \(N\ge 3\). For any \(i=1,...,k\), if \(y\in B_{{\frac{\mu r_3}{8k}}}(x_j)\) and \(j\ne i\), then
and
where \(A_{N,s}\) is a constant only depend on N and s. If \(y\in B_{{\frac{\mu r_3}{8k}}}(x_i)\), then
and
Proof
Let \({\bar{PU}}_{x_i,\Lambda }(x) = \mu ^{\frac{N-2s}{2}}PU_{x_i,\Lambda }(\mu x)\), then
So,
Case 1: \( y\in B_{\frac{r_3}{8k}}(\bar{x_i})\), it is easy to check
and
So,
That is, if \(y\in B_{{\frac{\mu r_3}{8k}}}({\bar{x}}_i)\), then
Case 2: \( y \in B_{{\frac{r_3}{8k}}}(\bar{x_j})\), where \( j\ne i\). In this case, it is easy to check
and
So,
That is, if \(y\in B_{{\frac{\mu \min (r_0,1)}{8k}}}(x_j)\), then
Since for \( l=1,...,N+1\),
Similar to (A.1) and (A.2), we can prove (A.3)-(A.6). \(\square \)
Appendix B. Energy expansion
In this section, we will give the expansion of the energy \(I(W_{r,\Lambda })\). Recall that \(\mu =k^{\frac{N-2s+1}{N-2s}}\), \( d=1-\frac{r}{\mu }\),
and
where \(PU_{x_j,\Lambda }(y) \) is the solution of (1.4).
Proposition B.1
If \(N\ge 3\) for \(\frac{3}{4} \le s<1\) and \(3\le N < 2s -1 +\frac{2}{3-4s} \) for \(\frac{11-\sqrt{41}}{8}< s<\frac{3}{4}\), then we have
where A, \(A_1\), \(A_2\), \(A_3\), \(B_1\) and \(B_2\) are positive constants.
Proof
By the symmetry, we have
where \( \bar{B_1} =\displaystyle \int _{{\mathbb {R}}^{N}} U_{x_1,\Lambda }^{2^{*}_s-1}. \)
Let
Then,
Note that for \(y \in \Omega _1\), \(|y-x_i|\ge |y-x_1|\). Thus
and
where \(\theta \) is a small positive constant. We can chose \(\theta \) small enough, then
On the other hand, it is easy to show that
and
Moreover
However,
Thus, we have proved
Combining (B.2) and (B.11), we can get
where A, \(B_1\) and \(B_2\) are positive constants.
Now, we estimate \(H( {\bar{x}}_1,{\bar{x}}_1)\) and \( G( {\bar{x}}_i,{\bar{x}}_1) \), \(i\ge 2\). Let \( {\bar{x}}_1^{*} = (\frac{1}{1-d},0,...,0 )\) be the reflection of \( {\bar{x}}_1 \) withe respect to the unit sphere. Then
We can compute that,
In fact, for \(i\le k^{\alpha }\), where \(\alpha \in (\frac{1}{N-2s-1},1)\) is a fix constant, we have
where \({\bar{O}}(f(i,k))\) means that, there is a constant C and \(k_0\) , for any \(k >k_0\) and any \( 2 \le i \le k^{\alpha } \),
On the other hand,
Noting \(N \ge 3\), by direct computation, we have
Since
and
it is easy to check
Combining (B.16) and (B.17), we have (B.14).
Finally, combining (B.12), (B.13) and (B.14), we get (B.1).\(\square \)
Proposition B.2
If \(N\ge 3\) for \(\frac{3}{4} \le s<1\) and \(3\le N < 2s -1 +\frac{2}{3-4s} \) for \(\frac{11-\sqrt{41}}{8}< s<\frac{3}{4}\), then we have
and
where \(A_1\), \(A_2\), \(A_3\), \(B_1\) and \(B_2\) are the same positive constants as in Proposition B.1.
Proof
We use \(\partial \) to denote either \(\frac{\partial }{\partial \Lambda }\) or \(\frac{\partial }{\partial d} \). Using the symmetry, we have
Then the proof of this proposition is similar to the proof of Proposition B.1, so we omit it. \(\square \)
Appendix C Basic estimates
In this section, we list some lemmas, whose proof can be found in [9] and [22].
For each fixed i and j, \(i \ne j\), consider the function
where \(\alpha \ge 1\) and \(\beta \ge 1\) are constants.
Lemma C.1
For any constant \(0< \sigma <\min (\alpha ,\beta )\), there is a constant \(C>0\), such that
Lemma C.2
For any constant \(0< \sigma <N-2s\), there is a constant \(C>0\), such that
Lemma C.3
Suppose that \(N\ge 3\), then there is a small \(\theta >0\), such that
where \( W_{r,\Lambda } = \sum _{j=1}^k PU_{x_j,\Lambda }.\)
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Guo, Y., hu, Y. & Liu, T. Non-radial solutions for the fractional Hénon equation with critical exponent. Calc. Var. 61, 172 (2022). https://doi.org/10.1007/s00526-022-02287-4
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DOI: https://doi.org/10.1007/s00526-022-02287-4