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arXiv 1206.5201math-phmath.APmath.MP
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星图上NLS方程驻波的变分性质和轨道稳定性

Variational properties and orbital stability of standing waves for NLS equation on a star graph

R. Adami, C. Cacciapuoti, D. Finco, D. Noja

摘要:

研究了星图{ $\mathcal{G}$ }上非线性薛定谔方程的驻波,星图{$N$}是由半直线组成的.在顶点处发生相互作用,该相互作用由强度为$α\leqslant 0$的δ型边界条件描述。非线性是聚焦功率型的。动力学由形式为$ i \frac{d}{dt}Ψ_t = H Ψ_t - | Ψ_t |^{2μ} Ψ_t $的方程给出,其中$H$是产生线性薛定谔动力学的哈密顿算子。我们表明存在的几个家庭的驻波的每一个符号的耦合在顶点的每一个$ω> \frac{α^2}{N^2}$。此外,我们确定的基态,作为最小化的Nehari流形上的行动,并命令的各个家庭。最后,我们表明,基态是轨道稳定的每个允许的$ω$,如果非线性是亚临界或临界的,否则为$ω<ω^\ast$。

英文摘要:

We study standing waves for a nonlinear Schrödinger equation on a star graph {$\mathcal{G}$} i.e. $N$ half-lines joined at a vertex. At the vertex an interaction occurs described by a boundary condition of delta type with strength $α\leqslant 0$. The nonlinearity is of focusing power type. The dynamics is given by an equation of the form $ i \frac{d}{dt}Ψ_t = H Ψ_t - | Ψ_t |^{2μ} Ψ_t $, where $H$ is the Hamiltonian operator which generates the linear Schrödinger dynamics. We show the existence of several families of standing waves for every sign of the coupling at the vertex for every $ω> \frac{α^2}{N^2}$. Furthermore, we determine the ground states, as minimizers of the action on the Nehari manifold, and order the various families. Finally, we show that the ground states are orbitally stable for every allowed $ω$ if the nonlinearity is subcritical or critical, and for $ω<ω^\ast$ otherwise.

机构、总结、中文摘要均由AI分析而来,可能存在错误,请以论文正文为准。

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