Failure of scattering for the NLSE with a point interaction in dimension two and three

C Cacciapuoti, D Finco, D Noja - Nonlinearity, 2023 - iopscience.iop.org
In this paper we consider the nonlinear Schrödinger (NLS) equation with power nonlinearity
and a point interaction (a'δ-potential'in the physical literature) in dimension two and three …

Global dynamics below a threshold for the nonlinear Schrödinger equations with the Kirchhoff boundary and the repulsive Dirac delta boundary on a star graph

M Hamano, M Ikeda, T Inui, I Shimizu - Partial Differential Equations and …, 2024 - Springer
We consider the nonlinear Schrödinger equations on the star graph with the Kirchhoff
boundary and the repulsive Dirac delta boundary at the origin. In the present paper, we …

Asymptotic behavior in time of solution for the cubic nonlinear Schrödinger equation on the tadpole graph

J Segata - Journal of Differential Equations, 2025 - Elsevier
The purpose of this paper is to study large time behavior of solution to the cubic nonlinear
Schrödinger equation on the tadpole graph which is a ring attached to a semi-infinite line …

A minimal mass blow-up solution on a nonlinear quantum star graph

F Genoud, SL Coz, J Royer - arXiv preprint arXiv:2302.09678, 2023 - arxiv.org
The main contribution of this article is the construction of a finite time blow-up solution to the
mass-critical focusing nonlinear Schr\" odinger equation set on a metric star graph $\mathcal …

Asymptotic behavior for the long-range nonlinear Schrödinger equation on the star graph with the Kirchhoff boundary condition

K Aoki, T Inui, H Miyazaki, H Mizutani, K Uriya - Pure and Applied Analysis, 2022 - msp.org
We consider the cubic nonlinear Schrödinger equation on the star graph with the Kirchhoff
boundary condition. We prove modified scattering for the final state problem and the initial …

PURE and APPLIED

K AOKI, T INUI, H MIYAZAKI, H MIZUTANI, K URIYA - projecteuclid.org
Background. We mainly consider the following cubic nonlinear Schrödinger equation (NLS)
on the star graph G with n-edges: i∂ t u+ K u+ λ| u| 2u= 0,(t, x)∈ I× G,(1-1) where I is a time …