Orbital instability of standing waves for NLS equation on star graphs
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Abstract:
We consider a nonlinear Schrödinger (NLS) equation with any positive power nonlinearity on a star graph $\Gamma$ ($N$ half-lines glued at the common vertex) with a $\delta$ interaction at the vertex. The strength of the interaction is defined by a fixed value $\alpha \in \mathbb {R}$. In the recent works of Adami et al., it was shown that for $\alpha \neq 0$ the NLS equation on $\Gamma$ admits the unique symmetric (with respect to permutation of edges) standing wave and that all other possible standing waves are nonsymmetric. Also, it was proved for $\alpha <0$ that in the NLS equation with a subcritical power-type nonlinearity, the unique symmetric standing wave is orbitally stable.
In this paper, we analyze stability of standing waves for both $\alpha <0$ and $\alpha >0$. By extending the Sturm theory to Schrödinger operators on the star graph, we give the explicit count of the Morse and degeneracy indices for each standing wave. For $\alpha <0$, we prove that all nonsymmetric standing waves in the NLS equation with any positive power nonlinearity are orbitally unstable. For $\alpha >0$, we prove the orbital instability of all standing waves.
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Additional Information
- Adilbek Kairzhan
- Affiliation: Department of Mathematics, McMaster University, Hamilton, Ontario, L8S 4K1, Canada
- MR Author ID: 1260013
- Email: kairzhaa@math.mcmaster.ca
- Received by editor(s): January 25, 2018
- Received by editor(s) in revised form: September 21, 2018
- Published electronically: March 15, 2019
- Communicated by: Catherine Sulem
- © Copyright 2019 American Mathematical Society
- Journal: Proc. Amer. Math. Soc. 147 (2019), 2911-2924
- MSC (2010): Primary 35Q55, 37K45; Secondary 35B35
- DOI: https://doi.org/10.1090/proc/14463
- MathSciNet review: 3973894