2018
DOI: 10.3934/dcds.2018221
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On the orbital instability of excited states for the NLS equation with the <i>δ</i>-interaction on a star graph

Abstract: We study the nonlinear Schrödinger equation (NLS) on a star graph G. At the vertex an interaction occurs described by a boundary condition of delta type with strength α ∈ R. We investigate the orbital instability of the standing waves e iωt Φ(x) of the NLS-δ equation with attractive power nonlinearity on G when the profile Φ(x) has mixed structure (i.e. has bumps and tails). In our approach we essentially use the extension theory of symmetric operators by Krein -von Neumann, and the analytic perturbations theo… Show more

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Cited by 36 publications
(48 citation statements)
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References 35 publications
(52 reference statements)
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“…See the proof of Lemma 2.3 in [6] (or Theorem 3.4 in [5]) for the detailed explanation of this fact.…”
Section: Well-posednessmentioning
confidence: 99%
“…See the proof of Lemma 2.3 in [6] (or Theorem 3.4 in [5]) for the detailed explanation of this fact.…”
Section: Well-posednessmentioning
confidence: 99%
“…The key point of this method is to use that the mapping datasolution associated to model (1) is at least of class C 2 (see Theorem 2.1 above). We note that the results in [35] have been applied successfully in the case of Schrödinger models on start graphs [10]- [11] and in [14]- [15] for models of KdV-type.…”
Section: Convexity Conditionmentioning
confidence: 99%
“…The case λ 2 = 0 and Z = 0 has been also studied substantially in the literature (see [3,8,12,16,20,22,23], [27,28,32,36,37] and references therein). The case of Schrödinger models on star graphs with δ conditions on the vertex also have been studied recently in Adami et.al ( [1,2] and references therein) and An-gulo&Goloshchapova ( [10,11,12]). The case of either other defect type or nonlinearity have been studied in [3,9,12,13,43].…”
mentioning
confidence: 99%
See 1 more Smart Citation
“…In the last years, the study of nonlinear dispersive models in a metric graph has attracted a lot of attention of mathematicians, physicists, chemists and engineers, see for details [9,10,14,34,35] and references therein. In particular, the framework prototype (graphgeometry) for description of these phenomena have been a star graph G, namely, on metric graphs with N half-lines of the form (0, +∞) connecting at a common vertex ν = 0, together with a nonlinear equation suitably defined on the edges such as the nonlinear Schrödinger equation (see Adami et al [1,2] and Angulo and Goloshchapova [5,6]). We note that with the introduction of nonlinearities in the dispersive models, the network provides a nice field, where one can look for interesting soliton propagation and nonlinear dynamics in general.…”
Section: Introductionmentioning
confidence: 99%