“…In the case λ < 0, stationary solutions are available, called Gaussons (as noticed in [14]; see below), which turn out to be orbitally stable, but not stable in the usual sense of Lyapunov [19,22] (see also [4] for another proof, and [44,46] for other particular solutions). In the case λ > 0, every solution is (global and) dispersive with a non-standard rate (a logarithmic perturbation of the Schrödinger rate), and after a time-dependent rescaling related to this dispersion, the large time behavior of the renormalized solution exhibits a universal Gaussian profile -a phenomenon which is rather unique in the context of Hamiltonian dispersive PDEs, see [17].…”