We consider a generalized nonlinear Schrödinger equation (NLS) with a power nonlinearity |ψ| 2μψ of focusing type describing propagation on the ramified structure given by N edges connected at a vertex (a star graph). To model the interaction at the junction, it is there imposed a boundary condition analogous to the δ potential of strength α on the line, including as a special case (α=0) the free propagation. We show that nonlinear stationary states describing solitons sitting at the vertex exist both for attractive (α<0, representing a potential well) and repulsive (α>0, a potential barrier) interaction. In the case of sufficiently strong attractive interaction at the vertex and power nonlinearity μ<2, including the standard cubic case, we characterize the ground state as minimizer of a constrained action and we discuss its orbital stability. Finally we show that in the free case, for even N only, the stationary states can be used to construct traveling waves on the graph
Adami, R., Cacciapuoti, C., Finco, D., Noja, D. (2012). Stationary states of NLS on star graphs. EUROPHYSICS LETTERS, 100(1) [10.1209/0295-5075/100/10003].
Stationary states of NLS on star graphs
NOJA, DIEGO DAVIDE
2012
Abstract
We consider a generalized nonlinear Schrödinger equation (NLS) with a power nonlinearity |ψ| 2μψ of focusing type describing propagation on the ramified structure given by N edges connected at a vertex (a star graph). To model the interaction at the junction, it is there imposed a boundary condition analogous to the δ potential of strength α on the line, including as a special case (α=0) the free propagation. We show that nonlinear stationary states describing solitons sitting at the vertex exist both for attractive (α<0, representing a potential well) and repulsive (α>0, a potential barrier) interaction. In the case of sufficiently strong attractive interaction at the vertex and power nonlinearity μ<2, including the standard cubic case, we characterize the ground state as minimizer of a constrained action and we discuss its orbital stability. Finally we show that in the free case, for even N only, the stationary states can be used to construct traveling waves on the graphFile | Dimensione | Formato | |
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