Abstract
The article is concerned with the existence of positive solutions of a semi-linear elliptic system defined in a cylinder \(\Omega =\Omega '\times (0,a)\subset {\mathbb {R}}^n\), where \(\Omega '\subset {\mathbb {R}}^{n-1}\) is a bounded and smooth domain. The system couples a superlinear equation defined in the whole cylinder \(\Omega \) with another superlinear (or linear) equation defined at the bottom of the cylinder \(\Omega '\times \{0\}\). Possible applications for such systems are interacting substances (gas in the cylinder and fluid at the bottom) or competing species in a cylindrical habitat (insects in the air and plants on the ground). We provide a priori \(L^\infty \) bounds for all positive solutions of the system when the nonlinear terms satisfy certain growth conditions. It is interesting that due to the structure of the system our growth restrictions are weaker than those of the pioneering result by Brezis–Turner for a single equation. Using the a priori bounds and topological arguments, we prove the existence of positive solutions for these particular semi-linear elliptic systems.
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1 Introduction
For scalar equations of the form
where \(\Omega \) is a smooth bounded domain of \({\mathbb {R}}^n\) and f(x, u) behaves like \(u^p\) for u large, the question of the existence of positive solutions has been intensively studied [2, 3, 11, 17, 20, 23]. One way to obtain existence results for (1.1) is using topological arguments especially when the equation has no variational structure. The main difficulty when using a topological approach lies in the need of obtaining a priori bounds. In recent years, several approaches have been developed to deal with this problem [3, 11, 17]. Subsequently, many existence results proved by a priori estimates for the scalar Eq. (1.1) have been extended to corresponding elliptic nonlinear coupled systems [4, 5, 12, 13, 15]. For instance, the following superlinear system
where \(\Omega \subset {\mathbb {R}}^n\) is a bounded domain and \(p, q>1\), is usually referred to as the coupled Lane-Emden system and has been widely investigated in the last few years (see [10, 16, 24] and the references therein). Such problems arise in the study of multicomponent reaction diffusion processes and in the modeling of several physical phenomena such as pattern formation and population evolution (see [25] and the references therein). The solutions in most of the cases represent densities and thus positive solutions of the systems are of particular interest. The exponents (p, q) in system (1.2) interplay, compensating each other, which play a crucial role in the questions of existence and nonexistence of positive solutions.
In [4], Clément, de Figueiredo and Mitidieri used a method which was developed in [11] for the case of one equation to obtain \(L^{\infty }\) a priori bounds. For another coupled system studied by de Figueiredo and Yang [15], the difficulties of obtaining a priori bounds were due to the presence of gradients in the nonlinear terms. The authors had to use some norm with weights depending on the distance to the boundary of the domain. They obtained a priori bounds via the so called blow-up method which was introduced by Gidas–Spruck [17] for the scalar case. In [5], the authors found \(L^\infty \) a priori bounds with different exponent assumptions imposed on the nonlinear terms; the technique used in their work is based on the work of Brezis and Turner [3] for one equation, in which they combined the Hardy–Sobolev inequality with interpolation techniques. In [5] the Brezis–Turner exponent assumption was replaced by conditions that involve two curves in the (p, q) plane. We remark that the method introduced by Brezie-Turner was the first general way to obtain uniform bounds of positive solutions and has become a classical way. Many other problems like reaction-diffusion systems and Ambrosetti-Prodi type problems have been solved by this method (see [14, 21]).
The objective of this paper is to study the existence of positive solutions of a particular semi-linear elliptic system defined in a cylinder \(\Omega =\Omega '\times (0,a)\subset {\mathbb {R}}^n\), where \(\Omega '\subset {\mathbb {R}}^{n-1}\) is a bounded and smooth domain. The system couples a superlinear equation defined in the whole cylinder \(\Omega \) with another superlinear (or linear) equation defined at the bottom \(\Omega '\times \{0\}\) of the cylinder. Possible applications for such systems are interacting substances (gas in the cylinder and fluid at the bottom) or competing species in a cylindrical habitat (insects in the air and plants on the ground). Extending the method of Brezis–Turner [3] to this kind of system, we provide a priori \(L^\infty \) bounds for all positive solutions when the nonlinear terms satisfy certain growth conditions. The approach we use consists of using the Hardy–Sobolev inequality and a suitable fixed point theorem. Unlike the setting in [3] where the nonlinear term f(x, u) is defined on \(\Omega \times {\mathbb {R}}\), in our framework f is non-local and we have to distinguish two cases, depending on the space dimension. It is interesting that due to the structure of the system our growth restrictions are weaker than those of the pioneering result by Brezis–Turner for a single equation. Using the a priori bounds and topological arguments, we prove the existence of positive solutions for these particular semi-linear elliptic systems.
2 The Main Result
In this paper we consider a system of equations on a cylindrical domain \(\Omega = \Omega '\times (0,a) \subset {\mathbb {R}}^n (n\ge 3)\), with \(x = (x',x_n) \in \Omega \) and \(\Omega ' \subset {\mathbb {R}}^{n-1}\) is smooth. The particularity of this system is that it couples two unknowns u(x) and \(v(x')\) which are defined on different domains. We can think of \(\Omega \) as a jar or a cylindrical habitat containing two interacting substances or species: the substance u(x) (say a gas, insects, birds...) is distributed in the interior of the jar or habitat \(\Omega \), while the substance \(v(x')\) (say a fluid, plants, worms...) is located at the bottom \(\Omega ' \times \{0\}\) of the jar or on the ground of the habitat. A simple model of such a time independent interacting system is
where \(\Delta _{(n)} = \sum _{i = 1}^n \frac{\partial ^2}{\partial x_i^2}\), \(x'=(x_1, \ldots , x_{n-1})\), \(\nu \) denotes the exterior normal to the boundary \(\partial \Omega \), and \(\gamma \), \(\eta \) are exponents with \(\gamma > 1\) and \( \eta \ge 1\).
Here, we assume that the vertically cumulated effect of the substance \(u(x), x\in \Omega \), interacts with the substance \(v(x')\) at the bottom \(\Omega '\), hence the term \(\int _0^a u^\eta (x',x_n)\, dx_n\) in the second equation; on the other hand, the substance \(v(x')\) at the bottom \(\Omega '\) interacts with the substance u(x) via a continuous coefficient function \(h: {\overline{\Omega }} \rightarrow {\mathbb {R}}^+\), which we may consider decreasing with increasing height \(x_n\).
The operator \(\Delta _{(n-1)}\) with Dirichlet boundary condition in the second equation is invertible, and we can insert the expression
into the first equation of the system, to obtain the non-local equation
Our aim is to prove the following result:
Theorem 2.1
Suppose that \(\Omega := \Omega '\times (0,a) \subset {\mathbb {R}}^n\) is a bounded open domain. Furthermore,
-
1)
if \(1 \le \eta <\frac{4n}{(n-1)(n-2)}\), then assume that \(1 < \gamma \eta \le \frac{2n+2}{n}\);
if \(\eta \ge \frac{4n}{(n-1)(n-2)}\), then assume that \(1<\gamma \eta \le \frac{n+1}{n-1}+\frac{2n\gamma }{(n-1)^2}\).
-
2)
\(h\in C({\overline{\Omega }}, {\mathbb {R}}^+)\), with \(h_m:= \min \{h(x), x \in {\overline{\Omega }}\} > 0\).
Then Eq. (2.2), and hence system (2.1), has a positive solution \(u\in W^{2,q}(\Omega ), 1\le q<\infty \).
Remark 2.1
Notice that for \(n=3, 4\), we are always in case 1), since then
The proof follows the ideas of the influential paper by Brezis–Turner [3], in which a single equation with a super-linear non-linearity was considered. It is interesting to note that the maximal exponent in the article of Brezis–Turner was \(\frac{n+1}{n-1}\). For \(\eta =1\), the maximal exponent for \(\gamma \) is
which is larger than \(\frac{n+1}{n-1}\), this is due to the regularizing effect of the inverted operator \((-\Delta _{(n-1)})^{-1}\).
We have not seen such type of coupled systems in the literature. Of course, one can consider many different versions of such couplings.
3 \(L^p\) regularity on the cylinder
The proof of Theorem 2.1 depends on a priori estimates of the solutions and a related existence theorem. The \(L^p\) theory presented here is to pave the way to get the a priori bound. In this part we will concentrate on showing that a weak solution of the equation
with \(f\in L^p(\Omega ) \ (1<p<\infty )\) will also be a strong solution which is twice weakly differentiable. The proof of the regularity is based on the a priori estimates below. In view of the mixed boundary conditions and the special shape of the domain, we will do an even reflection on the bottom of the cylinder to reduce the problem to a familiar case for which we can refer to the ninth chapter in [18].
3.1 \(L^p\) a priori estimate
We define the space \(H_{cyl}^1(\Omega )\) as the closure in \(H^1(\Omega )\) of the set \(C^1_{cyl}(\Omega )=\big \{u\in C^1(\Omega )\mid u(x)=0, \ x\in \partial \Omega '\times [0,a]\big \}\). Correspondingly, \(W^{1,p}_{cyl} =\{u\in W^{1,p}(\Omega )\mid u(x)=0, x\in \partial \Omega '\times [0,a]\ \}\).
Interior estimate:
Lemma 3.1.1
Assume that \(u\in W^{2,p}_{loc}(\Omega )\cap L^p(\Omega )\), \(1<p<\infty \), is a strong solution of the Eq. (3.1), then for \(f\in L^p(\Omega )\) and for any open domain \(\Omega _i\subset \subset \Omega \),
where \(C=C(n, p, \Omega _i, \Omega )\).
Since the interior estimate does not require the boundary condition, the proof of this lemma follows from the same proof of Theorem 9.11 [18].
Estimate on the bottom and the top:
Lemma 3.1.2
Assume that \(u\in W^{2,p}(\Omega )\), \(\Omega =\Omega '\times (0,a)\subset {\mathbb {R}}^n\), where \(\Omega '\subset {\mathbb {R}}^{n-1}\) is a bounded and smooth domain. \(1<p<\infty \) is a strong solution of (3.1), then for \(f\in L^p(\Omega )\) and for any open domain \(\Omega _b\subset \subset \Omega \cup \Big \{\Omega '\times \{0\}\Big \}\) or \(\Omega _t\subset \subset \Omega \cup \Big \{\Omega '\times \{a\}\Big \}\)
or
where \(C_b=C(n, p, \Omega _b, \Omega )\), \(C_t=C(n, p, \Omega _t, \Omega )\).
Proof
We extend u and f to \(\Omega '\times (-a,a)\) by even reflection, that is, by setting
for \(x_n<0\). It follows that the extended functions, say \({\tilde{u}}\) and \({\tilde{f}}\), satisfy the same equation of (3.1) weakly in \(\Omega '\times (-a,a)\). To prove this we take an arbitrary test function \(\varphi \in C_{cyl}^1(\Omega '\times (-a,a))\), then since u is a weak solution of (3.1) on \(\Omega \), we have
As \(\varphi \in C^1\) in \(\Omega '\times (0,a)\) and \(\varphi =0\) on \(\partial \Omega '\), we can take \(\phi =\varphi \) in \(\Omega '\times (0, a)\), then
On the other hand, due to the even reflection, from (3.3), we get
then taking \(\phi '=\varphi \) in \(\Omega '\times (-a,0)\), so
Consequently, we have
Besides, \({{\tilde{u}}}=0\), \(x\in \partial \Omega '\times [-a,a]\) and \(\frac{\partial {{\tilde{u}}}}{\partial x_n}\big |_{x_n=-a}=-\frac{\partial {{\tilde{u}}}}{\partial x_n}\big |_{x_n=a}=-\frac{\partial u}{\partial x_n}\big |_{x_n=a}=0\), so that \({{\tilde{u}}}\) is a weak solution of (3.1) in \(\Omega '\times (-a, a)\). By the evenness of \({\tilde{u}}\), we also have \(\frac{\partial {\tilde{u}}}{\partial x_n}\big |_{x_n=0}=0\). Then, for any open subset \({\widetilde{\Omega }}_b \subset \subset \Omega '\times (-a,a)\) we are able to apply the interior estimate and thus get the desired estimate for \({\widetilde{\Omega }}_b\) and hence also for \(\Omega _b:= {\widetilde{\Omega }}_b \cap \Omega \). \(\square \)
Estimate on the side:
Lemma 3.1.3
Assume that \(u\in W^{2,p}(\Omega )\), \(\Omega =\Omega '\times (0,a)\subset {\mathbb {R}}^n\), where \(\Omega '\subset {\mathbb {R}}^{n-1}\) is a bounded and smooth domain. \(1<p<\infty \) is a strong solution of (3.1) with \(u=0\) on \(\partial \Omega '\times [0,a]\), then for \(f\in L^p(\Omega )\) and for any open domain \(\Omega _s\subset \subset \{\overline{\Omega '}\times (0,a)\}\),
where \(C=C(n, p, \Omega _s, \Omega )\).
Proof
Since \(u(x)=0, x'\in \partial \Omega '\), the proof follows from the boundary \(L^p\) estimate of Theorem 9.13 [18]. \(\square \)
Estimate on the edge \((\partial \Omega '\times \{0,a\})\):
Lemma 3.1.4
Assume \(u\in W^{2,p}(\Omega )\), \(\Omega =\Omega '\times (0,a)\subset {\mathbb {R}}^n\), where \(\Omega '\subset {\mathbb {R}}^{n-1}\) is a bounded and smooth domain. \(1<p<\infty \), a strong solution of (3.1) with \(u=0\) on \(\partial \Omega '\times [0,a]\), then for \(f\in L^p(\Omega )\) and for any open domain \(\Omega _e\subset \subset \Omega \cup \big \{\overline{\Omega '}\times \{0\}\big \}\),
where \(C=C(n, p, \Omega _e, \Omega )\).
Proof
In the proof of Lemma 3.1.2, we extended u and f to \(\Omega '\times (-a,a)\) by even reflection, and we proved that the extended function \({\tilde{u}}\) is a weak solution of (3.1) in \(\Omega '\times (-a,a)\) with f replaced by \({\tilde{f}}\). In this case, each point \(x_0\in \partial \Omega '\times \{0\}\) is a boundary point of \(\Omega '\times (-a,a)\) on the side, we then can proceed as in the proof of Lemma 3.1.3 with \(\Omega _s\) replaced by \(\Omega _{S}\subset \subset \{\overline{\Omega '}\times (-a,a)\}\), since \(\Omega _e\subset \Omega _{S}\), we have
We therefore derive
\(\square \)
Combining all the estimates above, we get the following result.
Global \(L^p\) estimate and regularity:
Lemma 3.1.5
Assume that \(u\in W^{2,p}(\Omega )\cap W^{1,p}_{cyl}(\Omega )\), \(1<p<\infty \), satisfies (3.1); if \(f\in L^p (\Omega )\), then
where \(C=C(n, p, \Omega )\).
Proof
(see a similar proof of Theorem 2.2.3 [26]) From the boundary estimate we conclude that for \(x_0\in \partial \Omega \), there exists a neighborhood \(U(x_0)\) such that
According to Heine–Borel theorem, there exists a finite open covering \(U_1, \ldots , U_N\) to cover \(\partial \Omega \). Denote \(K=\Omega \setminus \mathop {\cup }\limits _{i=1}^NU_i\), then K is a closed subset of \(\Omega \) and there exists a subdomain \(U_0\subset \subset \Omega \) such that \(U_0\supset K\). Lemma 3.1.1 shows that
Using the theorem on the partition of unity, we can choose functions \(\eta _0, \eta _1, \ldots , \eta _N\) such that
Thus
\(\square \)
In the next lemma we eliminate the dependence of u on the right.
Lemma 3.1.6
(A better a priori \(L^P\) estimate, cf. [6], Lemma 3.2.1) Assume that \(u\in W^{2,p}(\Omega )\cap W^{1,p}_{cyl}(\Omega )\), \(2\le p<\infty \), satisfies (3.1), if \(f\in L^p (\Omega )\), then
where \(C=C(n, p, \Omega )\).
Proof
We argue by contradiction. If (3.10) is not true, then \(\forall N\), \(\exists {u_N}\in W^{2,p}(\Omega )\cap W^{1,p}_{cyl}(\Omega )\), \(f_N\in L^p(\Omega )\), such that
but
Let
then
and
From the global estimate Lemma 3.1.5 we have
taking \(N>C\), then
Following from Rellich–Kondrachov theorem (cf. [1], Theorem 6.3), \(W^{2,p}(\Omega )\hookrightarrow W^{1,p}(\Omega )\) compactly. That is there exists a sub-sequence such that
Since \(v_N\) satisfies (3.12) weakly, then
From (3.14), we have \(v_N\rightharpoonup v\) in \(W^{1,p}_{cyl}(\Omega )\), and hence
On the other hand, since
and (3.13), we see \(\Vert g_N\Vert _{L^p(\Omega )}\rightarrow 0\) as \(N\rightarrow \infty \), which implies \(\forall \varphi \in C^\infty _{cyl}(\Omega )\)
So,
as \(N\rightarrow \infty \) in (3.15). Hence v weakly satisfies
In the following we prove \(v=0\). Indeed, multiplying with v on both sides of Eq. (3.16), we get \(\int _{\Omega }|\nabla v|^2\, dx=0\), so \(\nabla v=0\), combining with the boundary condition then \(v=0\), which contradicts with \(\Vert v_N\Vert _{L^p(\Omega )}\rightarrow \Vert v\Vert _{L^p(\Omega )}=1\). \(\square \)
3.2 Regularity:
With the above a priori estimate we can get the following existence result:
Lemma 3.2.1
If \(f\in L^p(\Omega )\) with \(2\le p<\infty \), then the problem (3.1) has a unique strong solution \(u\in W^{2,p}(\Omega )\).
Proof
The existence of the strong solution follows as in Th.9.15 [18]. Here we present the main points of the proof. We start from the \(L^2\) regularity.
\(L^2\) interior regularity: If \(f\in L^2(\Omega )\), \(u\in H^1_{cyl}(\Omega )\) is a weak solution of (3.1), then \(u\in H^2_{loc}(\Omega )\cap W^{1,p}_{cyl}(\Omega )\), and for each open subset \(V\subset \subset \Omega \) we have the estimate
the constant C depending only on V, \(\Omega \). The proof of \(L^2\) interior regularity is the same as Theorem 1 ([8] section 6.3.1).
In order to get the boundary regularity, we extend u and f to \(\Omega '\times (-a,a)\) as we did in Lemma 3.1.2. The extended function \({\tilde{u}}\) and \({\tilde{f}}\) satisfy the same equation of (2.1) weakly in \(\Omega '\times (-a, a)\). Since the bottom \(\Omega '\times \{0\}\) is inside of \(\Omega '\times (-a,a)\) after the extension, then the proof of regularity near the bottom \(\Omega '\times \{0\}\) is the same as \(L^2\) interior regularity. Considering \(u=0\) on \(\partial \Omega '\), then the regularity near the side of the cylinder is the same as Theorem 4 ( [8] section 6.3.2). Thus we have:
\(L^2\) boundary regularity: If \(f\in L^2(\Omega )\), \(u\in H^1_{cyl}(\Omega )\) is a weak solution of (3.1), then \(u\in H^2(\Omega )\), and we have the estimate
the constant C depending only on \(\Omega \).
We are now in a position to prove Lemma 3.2.1 with \(2<p<\infty \). In fact, given that we have the same \(L^p\) a priori estimates as in chapter 9 [18], the interior regularity result follows directly from Lemma 9.16 [18]. After we did the even reflection, the case of local boundary regularity is handled similarly as the Lemma 9.16 as well.
For the uniqueness, assume \(u_1, u_2\in W^{2,p}(\Omega )\) both the strong solution of (3.1). Let \(u=u_1-u_2\), then \(u\in W^{2,p}(\Omega )\) and satisfy (3.16) weakly with v replaced by u. From Lemma 3.1.6,
therefore, \(u=0\) a.e. in \(\Omega \), that is, \(u_1=u_2\). \(\square \)
4 A Priori Bounds
In this section we will see that the growth conditions imposed on the nonlinear terms play an important role in acquiring a priori bounds for all positive solutions of system (2.1). These terms are embedded into different \(L^p\) spaces as the dimension n varies. Depending on the size of \(\eta \) (the growth of nonlinearity in u) we will find two different growth restrictions for \(\gamma \) (the growth of the nonlinearity in v).
First, we state the following Hardy-type estimate in \(H_{cyl}^1(\Omega )\), which is the preparatory step of the technical aspects of the proof. The constant C may change from line to line, we will use C for a generic constant.
Lemma 4.1
There exists \(C > 0\) such that for any \(u\in H^1_{cyl}(\Omega )\), we have
where \(\delta _{n-1}=\delta (x')\) denotes the distance of x to \(\partial \Omega ',\ \Omega '\subset {\mathbb {R}}^{n-1}\).
Proof
Notice that \(\displaystyle \int _{\Omega }\frac{u^2(x)}{\delta ^2(x')}\, dx=\int _0^a\int _{\Omega '}\frac{u^2(x)}{\delta ^2(x')}\, dx'dx_n\); we start the proof from the inner integral. Consider \(u_n\in C^\infty _{cyl}(\Omega )\); for fixed \(x_n\), \(u_n(x',x_n)\) is a function of \(x'\), then by Hardy’s inequality [22] we have
and then integrating along the \(x_n\) direction,
Since \(C^\infty _{cyl}(\Omega )\) is dense in \(H^1_{cyl}(\Omega )\), for \(u\in H^1_{cyl}(\Omega )\), there exists functions \(u_n(x)\in C^\infty _{cyl}(\Omega )\) such that
as \(n \rightarrow \infty \). This implies that \(\{u_n\}\) is a Cauchy sequence in \(H^1_{cyl}(\Omega )\), then there exist \(n_\epsilon \) such that for \(n, m\ge n_\epsilon \),
Notice \(u_n-u_m\in C^\infty _{cyl}(\Omega )\), we substitute \(u_n\) with \(u_n-u_m\) in (4.1), then
which implies that \(\big \{\frac{u_n(x)}{\delta (x')}\big \}\) is a Cauchy sequence in \(L^2(\Omega )\) and hence
for some \(y\in L^2(\Omega )\). It remains to show \(y=\frac{u(x)}{\delta (x')}\). Since \(\delta (x')\) is bounded, we have that
In fact,
and since \(u_n(x)\rightarrow u(x)\) in \(L^2(\Omega )\), we conclude that indeed \(y=\frac{u(x)}{\delta (x')}\). Then we complete the proof by letting \(n \rightarrow \infty \) in (4.1). \(\square \)
The next lemma is a variant of the Hardy-inequality.
Lemma 4.2
There exists \(C>0\) such that for \(n\ge 3\), and \(0\le \tau \le 1\), we have
where \(\displaystyle \frac{1}{q}=\frac{1}{2}-\frac{1-\tau }{n}.\)
Proof
By the Hölder inequality,
where \(\displaystyle \frac{1}{q}=\frac{1}{r}+\frac{1}{s}\) . We choose \(\displaystyle \tau r=2\) and \(\displaystyle \frac{1}{(1-\tau )s}=\frac{1}{2}-\frac{1}{n}\), thus
Applying Lemma 4.1 and Sobolev’s embedding theorem to the respective term in (4.2) we obtain
Then (4.3) becomes the desired inequality. \(\square \)
In what follows we let \(J_1'\) denote the first positive eigenfunction satisfying
where \(\lambda _1'\) is the first eigenvalue of \(-\Delta _{(n-1)}\) and \(J_1'\) is normalized so that \(\int _{\Omega '} |J_1'|^2\, dx'=1\). Furthermore, \(J_1(x)\) is the eigenfunction to the corresponding Laplacian equation in \(\Omega \), with \(J_1(x',x_n):= J_1'(x'), x_n \in (0,a)\), that is \(J_1(x',x_n)\) is constant in the variable \(x_n\) and satisfies
Remark 4.1
It is known that \(J_1'(x')>0\) in \(\Omega '\) and it follows from Hopf’s Lemma that \(J_1'(x')\ge C\delta _{n-1}(x')\) with \(C>0\). Note that \(\int _\Omega |J_1(x)|^2\, dx = a\).
The basic a priori bound we prove is the following.
Theorem 4.1
Suppose that \(h(x) \ge h_m > 0\). Furthermore,
-
if \(\displaystyle 1 \le \eta <\frac{4n}{(n-1)(n-2)}\ \), then suppose that \(1<\gamma \eta \le \frac{2n+2}{n};\)
-
if \(\displaystyle \eta \ge \frac{4n}{(n-1)(n-2)}\ \), then suppose that \( \displaystyle 1 < \gamma \eta \le \frac{n+1}{n-1}+\frac{2n\gamma }{(n-1)^2}\).
Then there is a constant K such that for any \(u\in H_{cyl}^1(\Omega )\) non-negative and satisfying weakly
then we have \(u\in {L^\infty }(\Omega )\) and
where K is independent of \(t\ge 0\).
We first prove some lemmas.
Lemma 4.3
Under the assumptions of Theorem 4.1, there is a constant \(K_1>0\) such that for any non-negative \(u\in H^1_{cyl}(\Omega )\) satisfying weakly Eq. (4.4) for some \(t\ge 0\), then we have
where \( f(x,u): =h(x)\big [(-\Delta _{(n-1)})^{-1}\left( \int _0^a u^\eta (x', x_n)\, dx_n\right) \big ]^\gamma \).
Proof
Since \(u\in H^1_{cyl}(\Omega )\) is a weak solution of (4.4), we have
Taking \(\varphi = J_1\) we get
Note that \(\partial \Omega = (\partial \Omega '\times [0,a]) \cup (\Omega ' \times \{0,a\})\). The left side of the equation yields, using that \(u|_{\partial \Omega '\times [0,a]} = 0\) and \(\partial _\nu J_1|_{\Omega ' \times \{0,a\}} = 0\)
Since by assumption h(x) has the positive lower bound \(h_m\), then
where \(k>0\) will be chosen below. Since we consider non-negative solutions, then \(\int _0^a u^\eta (x',x_n)\, dx_n\) is non-negative, and by the maximum principle, \((-\Delta _{(n-1)})^{-1}\left( \int _0^a u^\eta (x',x_n)\, dx_n\right) \) is non-negative. Therefore
Next, choose k such that \(h_m\cdot a\cdot k^{\gamma -1}\ge (\lambda _1')^2+1\), thus
Hence,
which implies t is bounded, and also
Since \(\displaystyle \lambda _1'\int _{\Omega }uJ_{1}\, dx=\int _{\Omega }f(x,u)J_{1}\, dx+t\int _{\Omega } |J_1|^2\, dx\), we see that also \(\displaystyle \int _{\Omega }f(x,u)J_{1}\, dx\) is bounded, and using Remark 4.1 we obtain,
This completes the proof of Lemma 4.3. \(\square \)
Next, we show a Poincaré type inequality in \(W^{1,p}_{cyl}(\Omega )\).
Lemma 4.4
There exists a constant \(C>0\) such that
Proof
We may assume \(u\in C^\infty _{cyl}(\Omega )\) and \((0,x_2,\dots ,x_n) \in \partial \Omega '\), then
therefore Hölder’s inequality yields
Taking the integration over \(\Omega \) on both sides, we get
and applying Fubini’s theorem to the right hand side of the inequality,
since \(\Omega '\) is bounded. Now assuming \(u_n \in C^{\infty }_{cyl}(\Omega )\) converging to u in \(W^{1,p}_{cyl}(\Omega )\), from the result above we have
Letting n go to infinity, we conclude that
\(\square \)
In the next Lemma we prove an \(H^1\)-a priori bound for any weak non-negative solution of Eq. (4.4).
Lemma 4.5
Under the assumptions of Theorem 4.1 there is a constant \(K_2\) such that
for every non-negative weak solution of Eq. (4.4).
Proof
Taking \(\varphi = u \in H^1_{cyl}(\Omega )\) in (4.5) we obtain
Applying the Hölder inequality and the Poincaré inequality in \(H^{1}_{cyl}(\Omega )\) to the second term on the right hand side we get
Next, for \(0<\alpha <1\), by Hölder’s inequality we get
We now distinguish the two cases:
Case 1: \(1\le \eta < \frac{4n}{(n-1)(n-2)}\)
We first show that for each \(\epsilon >0\) there is a \(C_\epsilon \) such that
where
In fact, since \(u\in H^1_{cyl}(\Omega )\), according to the Sobolev inequality, we know that \(u\in L^q(\Omega ), (q\le 2^*=\frac{2n}{n-2})\), and because
where \(\frac{1}{s}+\frac{1}{\theta }=1, (s, \theta >1)\) and \(s\eta \le 2^*\), we see that \(\int _{0}^{a}u^\eta \, dx_n\in L^{s}(\Omega ')\). Next, using that \((-\Delta _{(n-1)})^{-1}\) is a continuous operator from \(L^s(\Omega ') \rightarrow W^{2,s}(\Omega ')\), \(s\le \frac{2n}{n-2}\cdot \frac{1}{\eta }\), we are able to use the Morrey embedding inequality in \(\Omega '\subset {\mathbb {R}}^{n-1}\) and we have, for \(s>\frac{n-1}{2}\),
Therefore \(f(x,u)\in L^\infty (\Omega )\) for fixed \(u\in H^1_{cyl}(\Omega )\). Due to the condition of Theorem 2.1, it follows that \(1< \gamma < \beta _n\), and we conclude that
which means that for \(\epsilon > 0\) small, there exists \(M_\epsilon > 0\) such that \(\Vert f(x,u)\Vert _{L^{\infty }(\Omega )}\le \epsilon \Vert u\Vert ^{\beta _n\eta }_{L^{s\eta }(\Omega )}\), for \(\Vert u\Vert _{L^{s\eta }(\Omega )} \ge M_\epsilon \). This shows (4.9).
Next, with the aid of Lemma 4.3 and due to \((a+b)^l\le a^l+b^l\ (a, b\ge 0,\ 0<l<1)\), we deduce from (4.8)
Now we choose \(\displaystyle 0<\alpha =\frac{n+2}{2n+2}<1\), so that \(\displaystyle \beta _n\eta +\frac{1}{1-\alpha }=\frac{2}{1-\alpha }\). From (4.7), (4.8) and (4.13), we get by the Sobolev inequality for \(\Omega \subset {\mathbb {R}}^n\)
Applying Lemma 4.2 with \(\tau =\alpha \) we have
where \(\displaystyle \frac{1}{q}=\frac{1}{2}-\frac{1-\alpha }{n}\), i.e. \(\displaystyle q=\frac{1}{1-\alpha }\) by the choice of \(\alpha \) above. We can then conclude from (4.14) that
and the proof of Lemma 4.5 is complete in this case since also \(\Vert u\Vert _{L^2(\Omega )}\le C\) by Lemma 4.4 in \(H^{1}_{cyl}(\Omega )\). Note that the choice of s in (4.10) is possible for \(1\le \eta <\frac{4n}{(n-1)(n-2)}\).
Case 2: \(\eta \ge \frac{4n}{(n-1)(n-2)}\)
We show that for \(1\le \gamma <\beta _n:=\frac{n^2-1}{(n-1)^2\eta -2n}\)
where
Here denotes the critical Sobolev exponent for the embedding , \(\Omega '\subset {\mathbb {R}}^{n-1}\).
In fact, first \(u\in H^1_{cyl}(\Omega )\) which implies \(u\in L^\rho (\Omega )\), \(1\le \rho \le 2^*\cdot \frac{1}{\eta }\), then as in (4.11), \(\int _{0}^{a}u^\eta \, dx\in L^{\rho }(\Omega ')\). By \(L^p\) regularity in \(\Omega '\), we have \(v\in W^{2,\rho }(\Omega ')\). Then if , we again have \(\Vert v\Vert _{L^{\gamma \, r}(\Omega ')}\le C\Vert v\Vert _{W^{2,\rho }(\Omega ')}\) by the Sobolev embedding theorem. After this we have
Since \(\rho \le \frac{2^*}{\eta }\), we have \(f(x,u)\in L^r(\Omega )\) for fixed \(u\in H^1_{cyl}(\Omega )\) and
and hence, for \(1<\gamma \eta <\beta _n\eta \) and every \(\epsilon > 0\) there exists \(C_\epsilon \) such that
This shows (4.15).
From (4.8), (4.15), Lemma 4.3 and the Hölder inequality we now deduce
where \(\displaystyle \frac{1}{r}+\frac{1}{h}=1, r>1, h>1\). Again applying the Hardy inequality with \(\tau =\alpha \) we get
where \(\displaystyle \frac{1-\alpha }{h} = \frac{1}{2} - \frac{1-\alpha }{n}\), and thus \(\displaystyle 1-\alpha =\frac{nh}{2(n+h)}\). Since \(0<1-\alpha <1\), so \(\displaystyle 0<\frac{nh}{2(n+h)}<1\), which implies
Then as before, we take
Now that \(\displaystyle \rho \le \frac{2^*}{\eta }\), from (4.7), (4.19), (4.20) and (4.21) we get
We can then conclude from (4.22) that
Now combining (4.21) with and \(\gamma <\beta _n\), we are going to find a best r to have the largest \(\gamma \). So first we take \(\rho =\frac{2^*}{\eta }.\) Thus
Since \(\beta _n\) is increasing with respect to r and the largest \(\gamma \) is decreasing with respect to r, we can let
and derive
and thus, from (4.21)
Like the first case, the choice of \(\rho \) in (4.16) is possible for the second case of Theorem 2.1. Based on the above two cases (\(1\le \eta <\frac{4n}{(n-1)(n-2)}\), \(\eta \ge \frac{4n}{(n-1)(n-2)}\)), the proof of Lemma 4.5 is complete. \(\square \)
Proof of Theorem 4.1
Likewise, we consider two cases:
Case 1: \(1 \le \eta <\frac{4n}{(n-1)(n-2)}\), \(1 < \gamma \eta \le \frac{2n+2}{n}\).
By (4.12), we know \(f(x,u)\in L^\infty (\Omega )\) for any \(u\in H^1_{cyl}(\Omega )\) weak solution of (4.4). According to Lemma 3.2.1, for any fixed u, we have \(u\in W^{2,p}(\Omega )\), for any \(p>1\) and since \(J_1\) is a known smooth function, we have by Lemma 3.1.6 the estimate
Choosing \(p > \frac{n}{2}\), we get by Morrey’s inequality
In particular, due to (4.12) and Lemma 4.5, for \(\frac{n-1}{2} < s \le \frac{2^*}{\eta }\)
So that
Case 2: \(\eta \ge \frac{4n}{(n-1)(n-2)}\), \(1<\gamma \eta \le \frac{n+1}{n-1}+\frac{2n\gamma }{(n-1)^2}\).
Similarly, for any fixed \(u\in H^1_{cyl}(\Omega )\) weak solution of (4.4), according to (4.17), \(f(x,u)\in L^r(\Omega )\), so \(u\in W^{2,r}(\Omega )\) by Lemma 3.2.1, and by (3.10) with \(p=r\) we have
Next, we have by the Sobolev inequality that \(u\in L^\mu (\Omega )\), for \(\displaystyle \mu \le r^*=\frac{1}{\frac{1}{r}-\frac{2}{n}}=\frac{nr}{n-2r}\). By (4.17), (4.24) and the Sobolev embedding theorem
So finally we get
where \(2^*\le \mu \le r^*\).
For \(\frac{n}{r}=2\), we get \(\eta =\frac{4n}{n^2-5n+2}>\frac{4n}{(n-1)(n-2)}\), where r is given by (4.23). We denote this \(\eta \) as \(\eta '\). Hence when \(1\le \eta <\eta '\), thus \(2>\frac{n}{r}\), then Morrey’s embedding theorem implies \(r^*=\infty \), and then we are done.
Next, suppose that \(\eta '\le \eta \le 2^*\), it then follows that \(2\le \frac{n}{r}\). Then we will get an improved uniform \(L^p\) bound of f(x, u) by showing an improved uniform \(L^p\) bound of u. To see this we first consider
Similarly, in the case \(\displaystyle 2>\frac{(n-1)\eta }{r^*}\), we can replace by \(+\infty \). In the case \(\displaystyle 2\le \frac{(n-1)\eta }{r^*}\), we compute
From (4.25), we deduce
Noting that
hence
where the last inequality follows by elementary calculations, using (4.23). So we see that \(f(\cdot ,u)\) is bounded in an improved \(L^p\) space, if \(2\le \frac{(n-1)\eta }{r^*}\). Then taking , by (3.10) and the Sobolev inequality, we have,
where . From (4.27), we see , which means we get a better uniform \(L^p\) bound of u. Afterwards, we repeat the computation of (4.26) and get
Iterating (4.26)–(4.28), finally, we will derive
Thus, we have completed the proof of Theorem 4.1. \(\square \)
5 Fixed Point Theorem and Existence of the Solution
In this section we complete the proof of Theorem 2.1. We first show a maximum principle for the Poisson equation with mixed boundary conditions.
Lemma 5.1
([7]) Let \(\Omega \subset {\mathbb {R}}^n\), \(n\ge 3\), be the cylinder in (2.1) and let \( \Gamma _1\), \( \Gamma _2\) be a partition of \(\partial \Omega \), with \(\Gamma _1=\partial \Omega '\), \( \Gamma _2=\Omega '\times \{0, a\}\). Let \(g\in C_0^\infty (\Omega )\), \(g\ge 0\), \(g\not \equiv 0\), and let u denote the solution of
where \(\nu \) is the outer unit normal vector to \(\partial \Omega \). Then the solution of (5.1) satisfies:
Proof
If the claim were not true, then there exists a \(x_0\in {\overline{\Omega }}\) such that \(u(x_0)<0\). Without loss of generality, we suppose \(u(x_0)=\min \limits _{x\in {\overline{\Omega }}} u(x)<0\). By the assumption, we know \(x_0\notin {\Gamma _1}\). Next we show \(x_0\notin {\Gamma _2}\); otherwise, we may assume that \(x_0\in \Omega '\times \{0\}\) or \(\Omega '\times \{a\}\), by interior regularity, since \(g\in C^\infty _0(\Omega )\), we obtain \(u\in C^\infty (\Omega )\) and u in \(W^{2,p}(\Omega )\) (\(1\le p<\infty \)). In addition, \(W^{2,p}(\Omega )\hookrightarrow C^1({\bar{\Omega }})\) (for \(p>n\)) ( [1] Theorem 4.12, PART II), so we have \(u\in C^2(\Omega )\cap C^1({\bar{\Omega }})\). Since \(\Omega '\times \{0\}\) or \(\Omega '\times \{a\}\) is flat, \(\Omega \) satisfies the interior ball condition at \(x_0\), and from Hopf’s lemma we have \(\displaystyle \frac{\partial u(x_0)}{\partial \nu }<0\), which contradicts the assumption on \(\Gamma _2\). So \(x_0\) is an interior point of \(\Omega \). But due to the maximum principle, u cannot have a negative minimum in \(\Omega \). \(\square \)
We are now in the position to complete the proof of Theorem 2.1.
Proof of Theorem 2.1
For every fixed \(u\ge 0\) in \(C^1({{{\bar{\Omega }}}})\), by the Lax-Milgram theorem we know there exists a unique solution for Eq. (2.2), which we denote by \(w_u\). That is, \(-\Delta _{(n)} w_u=f(x,u)\), with \(f(x,u)= h(x)[(-\Delta _{(n-1)})^{-1}\int _0^a u^\eta (x)\, dx_n]^\gamma \). To solve problem (2.2), we define the mapping \(u\rightarrow w_u=: F(u)\). If there is a fixed point of F in \(C^1({{{\bar{\Omega }}}})\) such that \(F(u)=u\), we are done. Now we check that F satisfies the following fixed point theorem ( [9], Theorem 3.1; [19], Theorem 1).
F: \(C^1({{{\bar{\Omega }}}})\rightarrow C^1({{{\bar{\Omega }}}})\) a compact mapping, acting in the cone of non-negative functions, will have a fixed point u with \(0<r\le \Vert u\Vert _{C^1({{{\bar{\Omega }}}})}\le R<\infty \) provided
-
1)
\(Fu\ne s'u, s'\ge 1\) for \(\Vert u\Vert _{C^1({{{\bar{\Omega }}}})}=r\) and
-
2)
\(Fu\ne u-t\tilde{J_1}, t\ge 0\), for \(\Vert u\Vert _{C^1({{{\bar{\Omega }}}})}=R\),
where \({{\tilde{J}}}_1=(-\Delta _{(n)})^{-1} J_1\).
Step 1: \(F: C^1({{{\bar{\Omega }}}})\rightarrow C^1({{{\bar{\Omega }}}})\) is a compact mapping. It is easy to see that F is continuous, since it is a composition of continuous maps. Then, let \({\mathcal {A}}\subset C^1({{{\bar{\Omega }}}})\) be a bounded set, for \(u\in {\mathcal {A}}\) we have
thus \(f(x,u)\in L^\infty (\Omega )\) and \(\{f(x,u), u\in {\mathcal {A}}\}\) is uniformly bounded. Since \(-\Delta _{(n)} w_{u}=f(x,u)\), by Lemmas 3.1.6 and 3.2.1, \(w_{u}\in W^{2,q}(\Omega )\), q large enough, and lies in a bounded set in \(W^{2,q}(\Omega )\). Then by Morrey’s inequality, we get for \(q>n\), \(w_{u}\in C^{1, \gamma '}({{{\bar{\Omega }}}})\), that is
where \(\gamma '=1-\frac{n}{q}\). Therefore we have for every x, y in \({{{\bar{\Omega }}}}\), and \(\forall u\in {\mathcal {A}}\)
Hence, \(\forall \epsilon >0\), we take \(\delta =(\frac{\epsilon }{C})^{\gamma '/1}\) then, if \(|x-y|<\delta \), \(\{w_{u}\}\) satisfies
which means \(\{w_{u}, u\in {\mathcal {A}}\}\) is uniformly bounded and equicontinuous in \(C^1({{{\bar{\Omega }}}})\). According to the Arzelà-Ascoli theorem, it is in a compact set in \(C^{1}({{{\bar{\Omega }}}})\). Hence, F is a compact mapping from \(C^1({{{\bar{\Omega }}}})\) to \(C^1({{{\bar{\Omega }}}})\).
Step 2: F maps the non-negative cone in \(C^1({{{\bar{\Omega }}}})\) into itself. For this we are going to prove that when u is fixed non-negative, then \(w_u\) is non-negative. Indeed, \(w_u\) satisfies
where \(f(x,u)=f(x)=h(x)[(-\Delta _{(n-1)})^{-1}\int _0^au^\eta (x',x_n)dx_n]^\gamma \). By (5.2) \(f\in L^\infty (\Omega )\) so that \(f\in L^p(\Omega )\) for any \(p>1\) when u is fixed in \(C^1({{{\bar{\Omega }}}})\).
We assume
where \(f_n\in C_0^\infty (\Omega )\), \(f_n\ge 0\), \(\Vert f_n-f\Vert _{L^p(\Omega )}\rightarrow 0\ (1\le p<\infty )\). Applying Lemma 5.1, we get
On the other hand, subtracting (5.3) from (5.4), we get
Since \(f_n-f\in L^\infty (\Omega )\), by Lemma 3.2.1, we have \(w_{u_n}-w_{u}\in W^{2,p}(\Omega )\), p large enough. Then by Lemma 3.1.6 and Morrey’s inequality we have \(w_{u_n}-w_{u}\in C^{1,\gamma '}({{{\bar{\Omega }}}})\), and \(\Vert w_{u_n}-w_u\Vert _{C^{1,\gamma '}({{{\bar{\Omega }}}})}\le C\Vert w_{u_n}-w_u\Vert _{W^{2,p}(\Omega )}\le C\Vert f_n-f\Vert _{L^p(\Omega )}\) for \(p>n\). So, \(\Vert w_{u_n}-w_u\Vert _{C^{1,\gamma '}({{{\bar{\Omega }}}})}\le C\Vert f_n-f\Vert _{L^p(\Omega )}.\) Furthermore
which implies
so,
Since \(w_{u_n}\ge 0\), then \(w_u\ge 0\) in \({{\bar{\Omega }}}\).
Next we verify the two conditions (1) and (2).
(1) holds for \(r<(\frac{1}{C})^{\frac{1}{\gamma \eta -1}+1}\), where C will be determined later. If not, we suppose that there exists \(s'\ge 1\) and u with \(\Vert u\Vert _{C^1({{{\bar{\Omega }}}})}=r\) such that \(Fu=s'u\). Since \(-\Delta _{(n)} F(u)=f(x,u)\), we obtain
then
Multiplying by u and taking the integral over \(\Omega \) on both sides, we have,
Case 1: \(1 \le \eta <\frac{4n}{(n-1)(n-2)}\), \(1 < \gamma \eta \le \frac{2n+2}{n}\); by (5.5), Hölder inequality and (4.12) we get
From (4.10), the Sobolev embedding inequality and Lemma 4.4 we derive,
and hence
However, by assumption
which is a contradiction.
Case 2: \(\eta \ge \frac{4n}{(n-1)(n-2)}\), \(1<\gamma \eta \le \frac{n+1}{n-1}+\frac{2n\gamma }{(n-1)^2}\); from (4.18) and (5.5), we have
where \(\displaystyle \frac{1}{r}+\frac{1}{h}=1\). Moreover, since \(r>2\), so \(h<2< 2^*\). Then by the Sobolev embedding inequality, we have the same result as (5.6). Thus 1) will follow by the same proof.
For 2), we show that there exists \(R_1>0\) such that there is no solution of \(F(u)=u-t\tilde{J_1}\) with \(\Vert u\Vert _{C^1({{{\bar{\Omega }}}})}\ge R_1, \forall t\ge 0\). Indeed, suppose \(u\in H^1_{cyl}(\Omega )\) a solution of \(F(u)=u-t\tilde{J_1}\), then \(-\Delta _{(n)} F(u)=f(x,u)\), that is,
then by Theorem 4.1, \(\Vert u\Vert _{L^\infty (\Omega )}\le K\), K independent of \(t\ge 0\). We conclude that for any \(1<q<\infty \),
So for any \(R>R_1\), \(F(u)\ne u-t\tilde{J_1}\). \(\square \)
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Guo, Y., Ruf, B. A system of superlinear elliptic equations in a cylinder. Nonlinear Differ. Equ. Appl. 30, 62 (2023). https://doi.org/10.1007/s00030-023-00869-5
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DOI: https://doi.org/10.1007/s00030-023-00869-5