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Ground state sign-changing solutions for a class of double-phase problem in bounded domains
Boundary Value Problems volume 2020, Article number: 24 (2020)
Abstract
This paper is concerned with the following double-phase problem:
where \(N\geq2\) and \(1< p< q< N\). Assuming that the primitive of \(f(x,u)\) is asymptotically q-linear as \(|u|\rightarrow\infty\) and a weak version of Nehari-type monotonicity condition that the function \(u\mapsto\frac{f(x,u)}{|u|^{q-1}}\) is nondecreasing on \((-\infty,0) \cup(0,\infty)\) for a.e. \(x\in\varOmega\), we prove the existence of one ground state sign-changing solution via the constraint variational method and quantitative deformation lemma for the equation. Our results improve and generalize some results obtained by Liu and Dai (J. Differ. Equ. 265(9):4311–4334, 2018).
1 Introduction and main results
Differential equations and variational problems with double phase operator are a new and interesting topic. It arises from the nonlinear elasticity theory, strongly anisotropic materials, Lavrentiev’s phenomenon, and so on (see [2–5]). The study on double-phase problems attracts more and more interest in recent years, and many results have been obtained [1, 6–10]. More precisely, the research is related to the energy functional
where the integrand switches between two different elliptic behaviors. In [5], energies of the form (1) are used in the context of homogenization and elasticity, and the function a drives the geometry of a composite of two different materials with hardening powers p and q.
In this paper, we are concerned with the existence of sign-changing solutions of the double-phase problem

where Ω is a smooth bounded domain in \(\mathbb{R}^{N}\), \(N\geq 2\), \(1< p< q< N\), and
and \(f:\varOmega \times \mathbb{R}\mapsto \mathbb{R}\) is a Carathéodory function satisfying the following assumptions:
- \((h_{1})\):
\(f(x,t)=o(|t|^{p-2}t)\) as \(t\rightarrow 0\) uniformly in \(x\in \varOmega \);
- \((h_{2})\):
there exist \(q< r< p^{*}\) and some positive constant C such that
$$ \bigl\vert f(x,t) \bigr\vert \leq C\bigl(1 + \vert t \vert ^{r-1}\bigr), $$where \(p^{*} = \frac{Np}{N-p}\) is the critical exponent.
- \((h_{3})\):
\(\lim_{|t|\rightarrow +\infty } \frac{F(x,t)}{|t|^{q}} = +\infty \) uniformly in \(x\in \varOmega \), where \(F(x,t)=\int _{0}^{t}f(x,s)\,ds\);
- \((h_{4})\):
the function \(t\mapsto \frac{f(x,t)}{|t|^{q-1}}\) is nondecreasing on \((-\infty ,0)\cup (0,+\infty )\) for a.e. \(x\in \varOmega \).
The solution of (P) is understand in the weak sense, that is, \(u\in W_{0}^{1,H}(\varOmega )\) is a solution of (P) if
where \(W_{0}^{1,H}(\varOmega )\) will be defined in Sect. 2.
Note that energy functional φ associated with (P) is defined by
It is a well-known consequence of \((h_{1})\) and \((h_{2})\) that \(\varphi \in C^{1}(W_{0}^{1,H}(\varOmega ),\mathbb{R})\) and the critical points of φ are weak solutions of (P). Furthermore, if \(u\in W_{0}^{1,H}(\varOmega )\) is a solution of (P) and \(u^{\pm } \neq 0\), then u is a sign-changing solution of (P), where
To facilitate the narrative, we set
and put
Let us recall some previous results that led us to the present research. The first result is due to Perera and Squassina [6], who considered the following form of (P) with the q-superlinear nonlinearity:

Applying the Morse theory, they proved that (\(P_{1}\)) has a nontrivial solution by assuming that either
- \((T_{1})\):
\(\lambda \notin \{\lambda _{k}\}_{k=1}^{\infty }\); or
- \((T_{2})\):
for some \(\delta >0\), \(\frac{|t|^{r}}{r}+H(x,t)\leq 0\) for a.e. \(x\in \varOmega \) and \(|t|\leq \delta \); or
- \((T_{3})\):
\(\frac{|t|^{r}}{r}+H(x,t)\geq c|t|^{s}\) for a.e. \(x\in \varOmega \) and all \(t\in \mathbb{R}\) for some \(s\in (p,q)\) and \(c>0\).
Recently, Liu and Dai [1] investigated the sign-changing ground state solution of (P) under \((h_{1})\), \((h_{2})\), \((h_{3})\), and
- \((h_{4})'\):
the function \(t\mapsto \frac{f(x,t)}{|t|^{q-1}}\) is strictly increasing on \((-\infty ,0)\cup (0,+\infty )\).
Additionally, Liu and Dai [9] also obtained the existence of at least three ground state solutions of (P) by using the strong maximum principle for the homogeneous double-phase problem.
It is a well-known consequence of \((h_{4})'\) that there is unique \(t_{u}>0\) such that \(t_{u} u\in \mathbb{N}_{0}\) for every \(u\in W_{0} ^{1,H}(\varOmega )\setminus \{0\}\), which implies that φ has at most one minimizer on \(\mathbb{M}_{0}\). Moreover, \((h_{4})'\) plays a crucial role in [1]. In fact, condition \((h_{4})'\) implies that every minimizer of φ on \(\mathbb{M}_{0}\) is a critical point. However, if \(t\mapsto \frac{f(x,t)}{|t|^{q-1}}\) is nonstrictly increasing, then \(t_{u}\) and minimizer of φ on \(\mathbb{M} _{0}\) may not be unique, and their arguments become invalid.
Motivated by the aforementioned works, in the present paper, our goal is to generalize the results mentioned to (P) under a weaker assumption. Precisely, we obtain following results.
Theorem 1.1
Assume that\((h_{1})\)–\((h_{4})\)hold. Then problem (P) has a sign-changing solution\(u_{0}\in \mathbb{M}_{0}\)such that
Furthermore, suppose that
then\(u_{0}\)has precisely two nodal domains.
Theorem 1.2
Assume that\((h_{1})\)–\((h_{4})\)hold. Then\(m_{0}\geq 2n_{0}\).
The rest of this paper is organized as follows. In Sect. 2, we present some necessary preliminary knowledge on space \(W_{0}^{1,H}(\varOmega )\). In Sect. 3, we give some preliminary lemmas needed for the proofs of our main results. We complete the proofs of Theorems 1.1–1.2 in Sect. 4.
2 Preliminaries
To discuss problem (P), we need some facts on the space \(W_{0}^{1,H}( \varOmega )\), which is called the Musielak–Orlicz–Sobolev space. For this reason, we recall some properties involving the Musielak–Orlicz spaces, which can be found in [10–14] and references therein.
Denote by \(N(\varOmega )\) the set of all generalized N-functions. For \(1 < p < q\) and \(0\leq a(\cdot )\in L^{1}(\varOmega )\), we define
It is clear that \(H\in N(\varOmega )\) is locally integrable and
which is called condition \((\triangle _{2})\).
The Musielak–Orlicz space \(L^{H}(\varOmega )\) is defined by
endowed with the Luxemburg norm
The Musielak–Orlicz–Sobolev space \(W^{1, H}(\varOmega )\) is defined by
and is equipped with the norm
We denote by \(W_{0}^{1,H}(\varOmega )\) the completion of \(C_{0}^{\infty }(\varOmega )\) in \(W^{1,H}(\varOmega )\). With these norms, the spaces \(L^{H}(\varOmega )\), \(W_{0}^{1,H}(\varOmega )\) and \(W^{1,H}(\varOmega )\) are separable reflexive Banach spaces; see [10] for the details.
Proposition 2.1
([1, Proposition 2.1])
Set\(\rho _{H}(u)=\int _{ \varOmega }(|u|^{p}+a(x)|u|^{q})\,dx\). For\(u\in L^{H}(\varOmega )\), we have:
- (i)
For\(u\neq 0\), \(|u|_{H}=\lambda \Leftrightarrow \rho _{H}(\frac{u}{ \lambda })=1\);
- (ii)
\(|u|_{H}<1(=1; >1)\Leftrightarrow \rho _{H}(u)<1(=1; >1)\);
- (iii)
If\(|u|_{H}\geq 1\), then\(|u|^{p}_{H}\leq \rho _{H}(u)\leq |u|^{q} _{H}\);
- (iv)
If\(|u|_{H}\leq 1\), then\(|u|^{q}_{H}\leq \rho _{H}(u)\leq |u|^{p} _{H}\).
Proposition 2.2
([11, Propositions 2.15 and 2.18])
-
(1)
If\(1\leq \vartheta \leq p^{*}\), then the embedding from\(W_{0}^{1,H}(\varOmega )\)to\(L^{\vartheta }(\varOmega )\)is continuous. In particular, if\(\vartheta \in [1,p^{*})\), then the embedding\(W_{0}^{1,H}(\varOmega )\hookrightarrow L^{\vartheta }(\varOmega )\)is compact.
-
(2)
Assume that (2) holds. Then the Poincaré’s inequality holds, that is, there exists a positive constant\(C_{0}\)such that
$$ \vert u \vert _{H}\leq C_{0} \vert \nabla u \vert _{H},\quad u\in W_{0}^{1, H}(\varOmega ). $$
By this lemma there exists \(c_{\vartheta }> 0\) such that
where \(|u|_{s}\) denotes the usual norm in \(L^{\vartheta }(\varOmega )\) for \(1\leq \vartheta < p^{*}\). It follows from (2) of Proposition 2.2 that \(|\nabla u|_{H}\) is an equivalent norm in \(W_{0}^{1, H}(\varOmega )\). We will use the equivalent norm in the following discussion and write \(\|u\|=|\nabla u|_{H}\) for simplicity.
To discuss problem (P), we need to define a functional in \(W_{0}^{1,H}(\varOmega )\):
We know that (see [15, p. 63, example]) \(J\in C^{1}(W_{0}^{1,H}( \varOmega ),\mathbb{R})\) and the double-phase operator \(-\operatorname{div}(| \nabla u|^{p-2}\nabla u+a(x)|\nabla u|^{q-2}\nabla u)\) is the derivative operator of J in the weak sense. We denote \(L=J': W_{0}^{1,H}( \varOmega )\rightarrow (W_{0}^{1,H}(\varOmega ))^{*}\). Then
for all \(u, v\in W_{0}^{1,H}(\varOmega )\). Here \((W_{0}^{1,H}(\varOmega ))^{*}\) denotes the dual space of \(W_{0}^{1,H}( \varOmega )\), and \(\langle \cdot , \cdot \rangle \) denotes the pairing between \(W_{0}^{1,H}(\varOmega )\) and \((W_{0}^{1,H}(\varOmega ))^{*}\). Then we have the following:
Proposition 2.3
([1, Proposition 3.1])
Let\(E= W^{1,H}_{0}(\varOmega )\), and letLbe as before. Then
- (1)
\(L: E\rightarrow E^{*}\)a continuous, bounded, and strictly monotone operator.
- (2)
\(L: E\rightarrow E^{*}\)is a mapping of type\((S)_{+}\), that is, if\(u_{n}\rightharpoonup u\)inEand\(\limsup_{n\rightarrow +\infty }\langle L(u_{n})-L(u), u_{n}-u\rangle \leq 0\), then\(u_{n}\rightarrow u\)inE.
- (3)
\(L: E\rightarrow E^{*}\)is a homeomorphism.
3 Some preliminary lemmas
In this section, we give some preliminary lemmas crucial for proving our results.
Lemma 3.1
If assumptions\((h_{1})\)–\((h_{4})\)hold, then
where\(g(\tau )=\frac{1-\tau ^{p}}{p}-\frac{1-\tau ^{q}}{q}\), \(\tau \geq 0\).
Proof
By condition \((h_{4})\) we have
Clearly, \(g(t)\geq g(1)=0\) for any \(t\geq 0\). Hence from (6) it follows that
The proof is completed. □
From Lemma 3.1 we immediately have the following two corollaries.
Corollary 3.2
Assume that\((h_{1})\)–\((h_{4})\)hold. If\(u=u^{+}+u^{-}\in \mathbb{M}_{0}\), then
Corollary 3.3
Assume that\((h_{1})\)–\((h_{4})\)hold. If\(u\in \mathbb{N}_{0}\), then
Lemma 3.4
Assume that\((h_{1})\)–\((h_{3})\)and\((h_{4})'\)hold. If\(u\in E\)and\(u^{\pm }\neq 0\), then there exists a unique pair\((s_{u}, t_{u})\)of positive numbers such that
Proof
For any \(u\in E\) with \(u^{\pm }\neq 0\), we consider the functions \(g(s,t), h(s,t): [0,+\infty )\times [0,+\infty )\rightarrow \mathbb{R}\) given by
We directly compute that
Using assumptions \((h_{1})\) and \((h_{2})\), we deduce that, for any \(\varepsilon >0\), there is \(C_{\varepsilon }>0\) such that, for all \((x,t)\in \varOmega \times \mathbb{R}\),
where \(r\in [1,p^{*})\) was given in \((h_{2})\).
Thus, for \(s>0\) sufficiently small, by (8) and Proposition 2.2(2) we have
and
By (9), (10), and the arbitrariness of ε, it is easy to prove that \(g(s,s)>0\) and \(h(s,s)>0\) for \(s>0\) small.
Moreover, using (6), we have
Hence by (11) and \((h_{3})\) we have that, for \(s>1\),
and, for \(t>1\),
which yields that \(g(t,t)<0\) and \(h(t,t)<0\) for \(t>0\) large. Thus there are \(0< T< R\) such that
This fact, combined with (7), implies that
and
So, by the Miranda theorem in [16] we can find \((s_{u},t_{u}) \in (T,R)\times (T,R)\) such that \(g(s_{u},t_{u})=h(s_{u},t_{u})=0\). Therefore \(s_{u} u^{+}+t_{u} u^{-}\in \mathbb{M}_{0}\).
Next, we prove the uniqueness. Let \((s_{i}, t_{i})\) be such that \(s_{i} u^{+}+t_{i} u^{-}\in \mathbb{M}_{0}\), \(i=1,2\), that is,
Then from (5), (7), and (15) it follows that
and
Both (16) and (17) imply that \(s_{1}=s_{2}\) and \(t_{1}=t_{2}\), which in turn implies that \((s_{u},t_{u})\) is the unique pair of positive numbers such that \(s_{u} u^{+}+t_{u} u^{-}\in \mathbb{M}_{0}\). We end the proof. □
Furthermore we have the following:
Lemma 3.5
Assume that\((h_{1})\)–\((h_{3})\)and\((h_{4})'\)hold. Then
Proof
By Corollary 3.2 we conclude that
Moreover, for any \(u\in E\) with \(u^{\pm }\neq 0\), from Lemma 3.4 we deduce that
which implies
Therefore the conclusion directly follows from (18) and (19). □
Lemma 3.6
Assume that\((h_{1})\)–\((h_{3})\)and\((h_{4})'\)hold. Then\(m_{0}>0\)can be achieved.
Proof
Firstly, we will show that \(m_{0}>0\). Indeed, for every \(u\in \mathbb{M}_{0}\), we have \(u\in \mathbb{N}_{0}\) and \(\langle \varphi '(u),u\rangle =0\). Then by \((h_{1})\)–\((h_{2})\) and Propositions 2.1 and 2.2 we get
Thus, for any \(u\in \mathbb{N}_{0}\) with \(\|u\|<1\), we have that
which implies that
Therefore we obtain that \(m_{0}=\inf_{u\in \mathbb{M}_{0}} \varphi (u)\geq \alpha _{0}>0\).
It remains to prove that \(u_{0}\in \mathbb{M}_{0}\) and \(\varphi (u _{0})=m_{0}\). Let \(\{u_{n}\}\subset \mathbb{M}_{0}\) be a sequence of functions such that \(\varphi (u_{n})\rightarrow m_{0}\) as \(n\rightarrow +\infty \). Firstly, we claim that \(\{u_{n}\}\) is bounded. Suppose, by contradiction, that \(\|u_{n}\|\rightarrow +\infty \) and let \(v_{n}=\frac{u_{n}}{\|u_{n}\|}\). Without loss of generality, we may assume that \(v_{n}\rightharpoonup v\) in E. By the Sobolev embedding theorem we have
If \(v=0\), then \(v_{n}\rightarrow 0\) in \(L^{\vartheta }( \varOmega )\) for \(1\leq \vartheta < p^{*}\). Fix \(R>[q(m_{0}+1)]^{ \frac{1}{p}}(>1)\). By \((h_{1})\)–\((h_{2})\) there exists \(C_{1}>0\) such that
Then we have that
Let \(t_{n}=\frac{R}{\|u_{n}\|}\). Hence by (20) and Corollary 3.3 we get that
which yields a contradiction. Thus \(v\neq 0\).
For \(x\in \{y\in \mathbb{R}^{N}: v(y)\neq 0\}\), it is clear that \(\lim_{n\rightarrow +\infty }|u_{n}(x)|=+\infty \). By hypotheses \((h_{1})\) and \((h_{2})\) we can find \(C_{2}\in \mathbb{R}\) such that
Hence by using (21), \((h_{3})\), Proposition 2.1, and Fatou’s lemma we have
This contradiction shows that \(\{u_{n}\}\) is bounded in E. Going if necessary to a subsequence, we can assume that \(u_{n}^{\pm }\rightharpoonup u_{0}^{\pm }\) in E. Then \(u_{n}^{\pm }\rightarrow u_{0}^{\pm }\) in \(L^{\vartheta }(\varOmega )\) for \(\vartheta \in [1,p^{*})\) and \(u_{n}\rightarrow u_{0}\) a.e. on Ω.
Our next goal is to prove that \(u_{0}\in \mathbb{M}_{0}\) and \(\varphi (u_{0})=m_{0}\). Firstly, we claim that \(\inf_{u\in \mathbb{N}_{0}}\varphi (u)>0\). Indeed, for every \(u\in \mathbb{N}_{0}\), we have \(\langle \varphi '(u),u\rangle =0\). Then by \((h_{1})\), \((h_{2})\), and Propositions 2.1 and 2.2 we get
Thus, for any \(u\in \mathbb{N}_{0}\) with \(\|u\|<1\), we have that
which implies that \(\|u\|\geq \alpha _{0}\). This implies that \(\inf_{u\in \mathbb{N}_{0}}\varphi (u)>0\). Note that \(\{u_{n}\}_{n\in N}\subset \mathbb{M}_{0}\). Then it is obvious that \(\{u_{n}^{\pm }\}_{n\in N}\subset \mathbb{N}_{0}\), that is,
By \((h_{1})\) and \((h_{2})\), for any \(\varepsilon > 0\), there exists \(C_{\varepsilon }> 0\) such that
for all \((x,t)\in \varOmega \times \mathbb{R}\), where \(r\in [1,p^{*})\) was given in \((h_{2})\). Thus
Because of the boundedness of \(u_{n}\), there is \(C_{1}>0\) such that
Choosing \(\varepsilon =\frac{\min \{\alpha _{0}^{p},\alpha _{0}^{q}\}}{2C _{1}}\), we get
By the compactness of the embedding \(E\hookrightarrow L^{r}(\varOmega )\) for \(p< q< r< p^{*}\) we get
which yields \(u_{0}^{\pm }\neq 0\). Moreover, note that \(u_{n}^{\pm } \rightarrow u_{0}^{\pm }\) in \(L^{\vartheta }(\varOmega )\), \(\vartheta \in [1,p^{*})\). By conditions \((h_{1})\) and \((h_{2})\), combined with the Hölder inequality and Lebesgue theorem, we have
Hence by the weak lower semicontinuity of the norm we conclude that
because \(u_{n}^{\pm }\in \mathbb{N}_{0}\). Thus by Lemma 3.4 there exist \(s_{0}, t_{0}>0\) such that \(s_{0}u_{0}^{+}+t_{0}u_{0}^{-} \in \mathbb{M}_{0}\). Consequently, from (24) and Lemma 3.1 we have
This shows that
From this and from (25) we conclude that
□
Similarly to the proof of [1, Theorem 1.4], we can prove the following lemma.
Lemma 3.7
Assume that\((h_{1})\)–\((h_{3})\)and\((h_{4})'\)hold. If\(u_{0}\in \mathbb{M}_{0}\)and\(\varphi (u_{0})=m_{0}\), then\(u_{0}\)is a critical point ofφ.
Proof
It is clear that \(\langle \varphi '(u_{0}^{\pm }),u _{0}^{\pm }\rangle =0=\langle \varphi '(u_{0}),u_{0}^{\pm }\rangle \). It follows from assumption \((h_{4})'\) that, for \(0< s\neq 1\) and \(0< t\neq 1\),
If \(\varphi '(u_{0})\neq 0\), then there exist \(\delta >0\) and \(\nu >0\) such that
Let \(D=(\frac{1}{2},\frac{3}{2})\times (\frac{1}{2},\frac{3}{2})\) and \(g(s,t)=su_{0}^{+}+tu_{0}^{-}\). By (26) we have
Let \(\varepsilon :=\min \{\frac{m_{0}-\beta }{4},\frac{\lambda \delta }{8}\}\) and \(B(u,\delta ):=\{v\in E:\|v-u\|\leq \delta \}\). Then [17, Lemma 2.3] yields a deformation η such that
- (a)
\(\eta (1,v)=v\) if \(\varphi (v)< m_{0}-2\varepsilon \) or \(\varphi (v)>m _{0}+2\varepsilon \),
- (b)
\(\eta (1,\varphi ^{m_{0}+\varepsilon }\cap B(u,\delta ))\subset \varphi ^{m_{0}-\varepsilon }\), and
- (c)
\(\varphi (\eta (1,v))\leq \varphi (v)\) for all \(v\in E\),
where \(\varphi ^{m_{0}\pm \varepsilon }:=\{v\in E: \varphi (v)\leq m _{0}\pm \varepsilon \}\).
It is easy to see that
Next, we show that \(\eta (1,g(D))\cap \mathbb{M}_{0}\neq \emptyset \), contradicting the definition of \(m_{0}\). Let \(h(s,t)=\eta (1,g(s,t))\), \(\varphi _{0}(s,t)=\langle \varphi '(su_{0}^{+})u_{0}^{+}, \varphi '(su _{0}^{-})u_{0}^{-}\rangle \), and \(\varphi _{1}(s,t)=\langle \frac{1}{s}\varphi '(h^{+}(s,t)), \frac{1}{t}\varphi '(h^{-}(s,t)) \rangle \). Note that
Hence we have that \(\deg (\varphi _{0}, D, 0)=1\). On the other hand, using (27) and property (a) of η, we have that \(g=h\) on ∂D. Hence \(\varphi _{1}=\varphi _{0}\) on ∂D and \(\deg (\varphi _{1}, D, 0)=\deg (\varphi _{0}, D, 0)=1\). This show that \(\varphi _{1}(s,t)=0\) for some \((s,t)\in D\), and so \(\eta (1,g(s,t))=h(s,t) \in \mathbb{M}_{0}\). Therefore \(u_{0}\) is a critical point of φ. □
4 Sign-changing solutions
For any \(\lambda >0\), let \(f_{\lambda }(x,t)=f(x,t)+\lambda r|t|^{r-2}t\) and
Similarly, we define
and
Lemma 4.1
Assume that\((h_{1})\)–\((h_{4})\)hold. Then there exists a constant\(\alpha >0\), which does not depend on\(\lambda \in (0,1]\), such that
Proof
For any \(\varepsilon >0\), by \((h_{1})\), \((h_{2})\), and Propositions 2.1 and 2.2, for any \(\lambda \in (0,1]\) and \(u\in \mathbb{N}_{\lambda }\), we have
Thus for any \(u\in \mathbb{N}_{\lambda }\) with \(\|u\|<1\), we have that
which implies that
The proof is completed. □
Now we are ready to prove Theorem 1.1.
Proof of Theorem 1.1
Clearly, for every \(\lambda >0\), \(f_{\lambda }\) satisfies conditions \((h_{1})\)–\((h_{3})\) and \((h_{4})'\), and Lemmas 3.6 and 3.7 imply that there exists \(u_{\lambda }\in \mathbb{M}_{\lambda }\) such that
Furthermore, under assumptions \((h_{1})\)–\((h_{3})\), we easily obtain that \(\mathbb{M}_{0}\neq \emptyset \). Let \(v_{0}\in \mathbb{M}_{0}\). Then \(\varphi (v_{0}):=\kappa >0\) and \(\langle \varphi '(v_{0}),v_{0} ^{\pm }\rangle =0\). Therefore by Lemma 3.4 there exist \(s_{\lambda }>0\) and \(t_{\lambda }>0\) such that \(s_{\lambda }v_{0} ^{+}+t_{\lambda }v_{0}^{-}\in \mathbb{M}_{\lambda }\). Then from Corollary 3.2 and Lemma 4.1 we have
Hence, we can choose a sequence \(\{\lambda _{n}\}\) such that \(\lambda _{n}\rightarrow 0\) as \(n\rightarrow +\infty \) and
Thus we only need to prove the following claims to complete the proof of Theorem 1.1.
Claim 1
\(\{u_{\lambda _{n}}\}\)is bounded inE.
Arguing by contradiction, suppose that \(\|u_{\lambda _{n}}\|\rightarrow +\infty \) as \(n\rightarrow +\infty \). We define the sequence \(v_{n} =\frac{u_{\lambda _{n}}}{\|u_{\lambda _{n}}\|}\), \(n=1,2,\dots \). It is clear that \(\{v_{n}\}\subset E\) and \(\|v_{n}\|=1\) for any \(n\in N\). Therefore, going if necessary to a subsequence, we may assume that
If \(v=0\), then \(v_{n}\rightarrow 0\) in \(L^{\vartheta }(\varOmega )\) for \(1\leq \vartheta < p^{*}\). Fix \(R>[q(m_{0}+1)]^{\frac{1}{p}}\). Using conditions \((h_{1})\)–\((h_{2})\) and the Lebesgue dominated convergence theorem, we deduce that
for some constant \(C_{3}>0\).
Let \(t_{n}=\frac{R}{\|u_{n}\|}\). Then by (32) and Corollary 3.3 we get that
which yields a contradiction. Thus \(v\neq 0\).
By \((h_{3})\) we get
for all \(x\in \varOmega _{0}:=\{x\in \varOmega : v(x)\neq 0\}\). Therefore, using (21), (30), and Fatou’s lemma, we have
which is contradiction. The proof of Claim 1 is complete. Thus there exist a subsequence of \(\{\lambda _{n}\}\), still denoted by \(\{\lambda _{n}\}\), and \(u_{0}\in E\) such that
Claim 2
\(\varphi (u_{0})=m_{0}\)and\(\varphi '(u_{0})=0\).
By the Sobolev embedding theorem, \(u_{\lambda _{n}}\rightarrow u_{0} \) in \(L^{\vartheta }(\varOmega ), 1\leq \vartheta < p^{*}\), and \(u_{\lambda _{n}}(x)\rightarrow u_{0}(x)\) a.e. on Ω. By \((h_{2})\) and the Hölder inequality it is easy to directly compute that
where \(\frac{1}{r}+\frac{1}{r'}=1\). Then, using (30), (34), and \((h_{2})\), we deduce
Since L is of type \((S)_{+}\), we see that
and so \(u_{\lambda _{n}}^{\pm }\rightarrow u_{0}^{\pm }\) in E. Thus from (30) it follows that \(\varphi (u _{0})=\overline{m}\).
Moreover, by Proposition 2.3, (30), and (35) we get
This shows that \(\varphi '(u_{0})=0\). Again from Lemma 4.1 and (35) we have
This, together with (6) (\(t=0\)), shows that \(u_{0}^{\pm } \neq 0\). Therefore
Next, we will prove that \(\varphi (u_{0})= m_{0}\). Let ε be any positive number. Since \(m_{0}=\inf_{u\in \mathbb{M}_{0}} \varphi (u)\), there exists \(v_{\varepsilon }\in \mathbb{M}_{0}\) such that \(\varphi (v_{\varepsilon })< m_{0}+\varepsilon \). Then \((h_{3})\) implies that there exists \(M_{\varepsilon }>1\) such that, for \(s\geq M_{\varepsilon }\) or \(t\geq M_{\varepsilon }\),
In view of Lemma 3.4, there exists a pair \((s_{n},t_{n})\) of positive numbers such that \(s_{n}v_{\varepsilon }^{+}+t_{n}v_{\varepsilon }^{-}\in \mathbb{M}_{\lambda _{n}}\), which, together with (38), implies \(0< s_{n}\), \(t_{n}< M_{\varepsilon }\). Thus from Lemma 3.1 and \(\langle \varphi '(v_{\varepsilon }),v_{\varepsilon }^{\pm }\rangle =0\) we have
which yields
Since \(\varepsilon > 0\) is arbitrary, we have \(\overline{m}\leq m_{0}\). Thus \(\overline{m}= m_{0}\), that is, \(\varphi (u_{0})=m_{0}\).
Now we show that \(u_{0}\) has exactly two nodal domains. Let \(u_{0}=u_{1}+u_{2}+u_{3}\), where
and \(\varOmega _{i}\) (\(i=1,2\)) are connected open subsets of Ω.
Setting \(v=u_{1}+u_{2}\), we see that \(v^{+}=u_{1}\) and \(v^{-}=u_{2}\), that is, \(v^{\pm }\neq 0\). Noting that \(\varphi '(u_{0})=0\), by a simple computation we have
By Lemma 3.1 and again by (40) and (41) we conclude that
which, together with (3), shows that \(u_{3}=0\). Therefore \(u_{0}\) has exactly two nodal domains. □
Proof of Theorem 1.2
By Theorem 1.1 there exists \(u_{0}\in \mathbb{M}_{0}\) such that \(\varphi (u_{0})=m_{0}\). Since \(u_{0}^{\pm }\in \mathbb{N}_{0}\), we have \(m_{0}=\varphi (u_{0})= \varphi (u_{0}^{+})+\varphi (u_{0}^{-})\geq 2n_{0}\). □
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This work is supported by the Fundamental Research Funds for the Central Universities (No. 3072019CF2402), the National Natural Science Foundation of China (No. 11201095), the Postdoctoral research startup foundation of Heilongjiang (No. LBH-Q14044), and the Science Research Funds for Overseas Returned Chinese Scholars of Heilongjiang Province (No. LC201502).
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Hou, G., Ge, B., Zhang, B. et al. Ground state sign-changing solutions for a class of double-phase problem in bounded domains. Bound Value Probl 2020, 24 (2020). https://doi.org/10.1186/s13661-020-01333-4
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DOI: https://doi.org/10.1186/s13661-020-01333-4