Abstract
We study the nonlinear Schrödinger equation with an arbitrary real potential \(V(x)\in (L^1+L^\infty )(\Gamma )\) on a star graph \(\Gamma \). At the vertex an interaction occurs described by the generalized Kirchhoff condition with strength \(-\gamma <0\). We show the existence of ground states \(\varphi _{\omega }(x)\) as minimizers of the action functional on the Nehari manifold under additional negativity and decay conditions on V(x). Moreover, for \(V(x)=-\dfrac{\beta }{x^{\alpha }}\), in the supercritical case, we prove that the standing waves \(e^{i\omega t}\varphi _{\omega }(x)\) are orbitally unstable in \(H^{1}(\Gamma )\) when \(\omega \) is large enough. Analogous result holds for an arbitrary \(\gamma \in {\mathbb {R}}\) when the standing waves have symmetric profile.
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29 April 2021
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Acknowledgements
The authors are kindly grateful to Prof. Gláucio Terra for the proof of Remark 1.2.
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Appendix
Appendix
Below we show some properties of the operator \( H_{\gamma , V}\) introduced by (1.2).
Lemma 4.10
Let \(\gamma \in {\mathbb {R}}\) and \(V(x)=\overline{V(x)}\in L^{1}(\Gamma )+L^{\infty }(\Gamma )\). The quadratic form \( {F}_{\gamma , V}\) given by (1.3) is semibounded and closed, and the operator \( H_{\gamma , V}\) defined by
is the self-adjoint operator associated with \( {F}_{\gamma , V}\) in \(L^{2}(\Gamma )\).
Proof
We can write \(V(x)=V_{1}(x)+V_{2}(x)\), with \(V_{1}\in L^{1}(\Gamma )\) and \(V_{2}\in L^{\infty }(\Gamma )\). Thus, using the Gagliardo–Nirenberg inequality (see formula (2.1) in [10]) and the Young inequality, we have
Similarly, by the Sobolev embedding, we obtain
Therefore,
Then, by the KLMN theorem [26, Theorem X.17], we infer that the quadratic form \( {F}_{\gamma , V}\) is associated with a semibounded self-adjoint operator \( T_{\gamma , V}\) defined by (observe that \(A=H_{0,0}\) in [26, Theorem X.17], i.e., \(V\equiv 0, \gamma =0\))
It is easily seen that \({\hbox {dom}}( H_{\gamma , V})\subseteq {\hbox {dom}}( T_{\gamma , V})\) and \( T_{\gamma , V}u= H_{\gamma , V}u, \,\,u\in {\hbox {dom}}( H_{\gamma , V})\). Hence, it is sufficient to prove that \({\hbox {dom}}( T_{\gamma , V})\subseteq {\hbox {dom}}( H_{\gamma , V})\).
Let \(\tilde{u}\in {\hbox {dom}}( T_{\gamma , V})\) and \(\tilde{v}\in H^1(\Gamma )\), then there exists \(\tilde{y}\in L^{2}(\Gamma )\) such that
Observe that \(\tilde{y}-V\tilde{u}\in L^1_{loc}(\Gamma )\) and set
Suppose now additionally that \(\tilde{v}\) has a compact support, then
From (4.20), we deduce
Combining (4.21) and (4.22), we get
Choose \(\tilde{v}=(\tilde{v}_e)_{e=1}^N\) such that \(\tilde{v}_1(x)\in C_0^\infty ({\mathbb {R}}^+)\) and \(\tilde{v}_2(x)\equiv \ldots \equiv \tilde{v}_N(x)\equiv 0.\) Then we obtain
therefore \(\tilde{u}'_1+z_1\equiv const\equiv c_1\). We have used that \(\tilde{u}'_1+z_1\in \mathrm {Ran}(A)^{\perp },\) where \(Av=v'\) with \({\hbox {dom}}(A)=C_0^\infty ({\mathbb {R}}^+)\) in \(L^{2}({\mathbb {R}}^+)\). Analogously \(\tilde{u}'_e+z_e\equiv const\equiv c_e,\,\, e=2,\ldots , N. \) Finally, from (4.23) we deduce
Assuming that \(\tilde{v}_1(0)\ne 0,\) we arrive at \(\sum \limits _{e=1}^N\tilde{u}'_e(0)=-\gamma \tilde{u}_1(0).\) Moreover, \(-\tilde{u}''+V\tilde{u}=z'+V\tilde{u}=\tilde{y}-V\tilde{u}+V\tilde{u}=\tilde{y}\in L^{2}(\Gamma ).\) Hence, \(\tilde{u}\in {\hbox {dom}}( H_{\gamma , V})\) and \({\hbox {dom}}( T_{\gamma , V})\subseteq {\hbox {dom}}(H_{\gamma , V}).\) \(\square \)
Lemma 4.11
Suppose that \(V(x)=\overline{V(x)}\in L^{2}_{\varepsilon }(\Gamma )+L^\infty (\Gamma )\), i.e., for any \(\varepsilon >0\) and \(V\in L^{2}_{\varepsilon }(\Gamma )+L^\infty (\Gamma )\) there exists a representation \(V=V_1+V_2, \, V_1\in L^{2}(\Gamma ), V_2\in L^{\infty }(\Gamma )\), with \(\Vert V_1\Vert _2^{2}\le \varepsilon \). Then, we have
Moreover, for m sufficiently large, \( H_{\gamma , V}\)-norm \(\Vert (H_{\gamma , V}+m)\cdot \Vert _2\) is equivalent to \(H^{2}\)-norm on \(\Gamma .\)
Proof
Observe that, by \( V(x)\in L^{2}_{\varepsilon }(\Gamma )+L^\infty (\Gamma )\), the Sobolev and the Young inequalities we get
and
It is immediate from (4.25), (4.26) that
And for m sufficiently large, inequalities (4.25) and (4.26) imply
Thus, we get (4.24).
The second assertion follows from (4.27),(4.28), and
\(\square \)
Remark 4.12
Observe that there exists potential V(x) satisfying Assumptions 1–4 such that \({\hbox {dom}}( H_{\gamma , V})\ne D_{H^{2}}.\) For example, consider \(V(x)=-1/x^\alpha ,\,1/2\le \alpha <1,\) and \(N=\gamma =2\), then \(v=(e^{-x}, e^{-x})\in D_{H^{2}}\), but
Lemma 4.13
Let \(\gamma >0\) and \(V(x)=\overline{V(x)}\) satisfy Assumptions 1–3. Then, the following assertions hold.
(i) The number \(-\omega _0\) defined by (1.5) is negative.
(ii) Let also \(m>\omega _0\), then \(\sqrt{ {F}_{\gamma , V}(v)+m\Vert v\Vert _2^{2}}\) defines a norm equivalent to the \(H^1\)-norm.
(iii) The number \(-\omega _0\) is the first eigenvalue of \(H_{\gamma , V}\). Moreover, it is simple, and there exists the corresponding positive eigenfunction \(\psi _0\in {\hbox {dom}}(H_{\gamma , V})\), i.e., \(H_{\gamma , V}\psi _0=-\omega _0\psi _0.\)
Proof
(i) To show \(-\omega _0<0\), observe that
Consider \(v^{\lambda }(x)=\lambda ^{\frac{1}{2}}v(\lambda x)\) with \(\lambda >0\). Hence,
For \(\lambda \) small enough, we have \( {F}_{\gamma , V}(v^{\lambda })<0\). Finally, \(-\omega _0\) is finite since \({F}_{\gamma , V}(v)\) is lower semibounded.
(ii) Let \(\varepsilon >0\). Firstly, notice that from (4.19) one easily gets
Secondly, for \(\varepsilon \) and \(\delta \) sufficiently small,
Indeed, the family of sesquilinear forms
is holomorphic of type (a) in the sense of Kato in the complex neighborhood of zero (see [21, Chapter VII, §4] for the definition and [21, Chapter VI, §1, Example 1.7] for the proof of sectoriality). Using inequality (4.7) in [21, Chapter VII] with \(\kappa =\kappa _2=0, \kappa _1=\delta \), we obtain \(|{\mathrm {t}}(\delta )[v]-{\mathrm {t}}(0)[v]|\le \varepsilon |{\mathrm {t}}(0)[v]|.\) Hence,
(iii) Step 1. Let \(\{v_{n}\}\) be a minimizing sequence, that is, \({F}_{\gamma , V}(v_{n})\underset{n\rightarrow \infty }{\longrightarrow } -\omega _{0}\), \(\left\| v_{n}\right\| ^{2}_2=1\) for all \(n\in \mathbb {N}\). From (ii), we deduce that \(\{v_{n}\}\) is bounded in \(H^{1}(\Gamma )\). Then, there exist a subsequence \(\{v_{n_k}\}\) of \(\{v_n\}\) and \(v_0\in H^{1}(\Gamma )\) such that \(\{v_{n_k}\}\) converges weakly to \(v_0\) in \(H^1(\Gamma )\). Observe that, by the weak lower semicontinuity of \(L^{2}\)-norm and \({F}_{\gamma , V}(\cdot )\), we get \(\left\| v_0\right\| _2\le 1\) and
We have \(\left\| v_0\right\| _{2}=1\), since, otherwise, there would exist \(\lambda >1\) such that \(\left\| \lambda v_0\right\| _{2}=1\) and \(F_{\gamma , V}(\lambda v_0)=\lambda ^{2}F_{\gamma , V}(v_0)<-\omega _0\), which is a contradiction. Consequently, \(v_0\) is a minimizer for (4.29).
Let \(\psi _{0}=\left| v_0\right| \), then \(\psi _{0}\ge 0\) on \(\Gamma \) and \(\left\| \psi _{0}\right\| ^{2}_2=\left\| v_{0}\right\| ^{2}_2=1\). Notice that \( \left\| \psi '_{0}\right\| ^{2}_2\le \left\| v'_0\right\| ^{2}_2,\) therefore \({F}_{\gamma , V}(\psi _{0})\le {F}_{\gamma , V}(v_0)\). Then, \(\psi _{0}\) is a minimizer of (4.29). This implies the existence of the Lagrange multiplier \(-\mu \) such that
Repeating the arguments from the proof of [2, Theorem 4], we get \(\psi _0\in {\hbox {dom}}(H_{\gamma , V})\) and
Multiplying the above equation by \(\overline{\psi _0}\) and integrating, we conclude \(\mu =\omega _0.\) Recalling that \(V(x)\le 0\) a.e. on \(\Gamma \), and arguing as in the proof of Proposition 1.1, one can show that \(\psi _0>0\) on \(\Gamma .\) Notice that one needs to apply [28, Theorem 1] with \(\beta (s)=\omega _0 s.\)
Step 2. Suppose that \(u_0\) is a nonnegative solution of
Let us show that there exists \(C>0\) such that \(u_0(x)=C\psi _0(x)\). Assume that this is false. Then, there exists \(C>0\) such that \(\widetilde{u}_0(x)=u_0(x)-C\psi _0(x)\) takes both positive and negative values. We have \(H_{\gamma , V}\widetilde{u}_0=-\omega _0 \widetilde{u}_0;\) consequently, \(\widetilde{v}_0=\widetilde{u}_0/\Vert \widetilde{u}_0\Vert _2\) is the minimizer of (4.29). Arguing as in Step 1, one can show that \(|\widetilde{v}_0|\) is also a minimizer and \(|\widetilde{v}_0|>0\). Therefore, \(\widetilde{u}_0(x)\) has a constant sign. This is a contradiction.
Suppose now that \(u_0\) is an arbitrary solution to (4.30) such that \(\Vert u_0\Vert _2^{2}=1\) (that is, \(u_0\) is a minimizer of (4.29)). Define \(w_0=|{\hbox {Re}}u_0|+i|{\hbox {Im}}u_0|,\) then \(|w_0|=|u_0|\) and \(|w'_0|=|u'_0|\); consequently, \(F_{\gamma , V}(u_0)=F_{\gamma , V}(w_0)\) and \(\Vert w_0\Vert _2^{2}=1.\) Therefore, \(w_0\) is a minimizer of (4.29). This implies that \(w_0\) satisfies (4.30), and, in particular, \(|{\hbox {Re}}u_0|\) and \(|{\hbox {Im}}u_0|\) satisfy (4.30). Thus, \(|{\hbox {Re}}u_0|=C_1 \psi _0\) and \(|{\hbox {Im}}u_0|=C_2\psi _0,\, C_1,C_2>0\); consequently, \({\hbox {Re}}u_0=\widetilde{C}_1 \psi _0\) and \({\hbox {Im}}u_0=\widetilde{C}_2\psi _0,\, \widetilde{C}_1,\widetilde{C}_2\in {\mathbb {R}},\) since \({\hbox {Re}}u_0\) and \({\hbox {Im}}u_0\) do not change the sign. Finally, \(u_0=\widetilde{C}_1\psi _0+i\widetilde{C}_2\psi _0=\widetilde{C}\psi _0, \, \widetilde{C}\in {\mathbb {C}},\) and therefore, \(-\omega _0\) is simple.
\(\square \)
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Ardila, A.H., Cely, L. & Goloshchapova, N. Instability of ground states for the NLS equation with potential on the star graph. J. Evol. Equ. 21, 3703–3732 (2021). https://doi.org/10.1007/s00028-021-00670-w
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DOI: https://doi.org/10.1007/s00028-021-00670-w
Keywords
- Nonlinear Schrödinger equation
- Linear potential
- Generalized Kirchhoff’s condition
- Ground state
- Orbital stability