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20012009
most citedGlobal well-posedness and scattering for the energy-critical nonlinear Schrödinger equation in R^3

51 citations · 98 across the 16 of their papers we have counts for

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Showing 2002 · math.APShow all

7 papers · 2 filters

math.AP2002

Polynomial upper bounds for the instability of the Nonlinear Schrödinger equation below the energy norm

J. Colliander, M. Keel, G. Staffilani +2

We continue the study (initiated in \cite{ckstt:7}) of the orbital stability of the ground state cylinder for focussing non-linear Schrödinger equations in the norm for…

math.AP2002

Local well-posedness for dispersion generalized Benjamin-Ono equations

J. Colliander, C. Kenig, G. Staffilani

In this paper we study local well-posedness in the energy space for a family of dispersive equations that can be seen as dispersive ``interpolations'' between the KdV and the Benja…

math.AP20021 cited

Polynomial upper bounds for the orbital instability of the 1D cubic NLS below the energy norm

Jim Colliander, Mark Keel, Gigliola Staffilani +2

We study the long-time behaviour of the focusing cubic NLS on in the Sobolev norms for . We obtain polynomial growth-type upper bounds on the norms, and…

math.AP2002

Low regularity solutions for the Kadomtsev-Petviashvili I equation

J. Colliander, C. Kenig, G. Staffilani

In this paper we obtain local in time existence and (suitable) uniqueness and continuous dependence for the KP-I equation for small data in the intersection of the energy space and…

math.AP2002

KdV and Almost Conservation Laws

Gigliola Staffilani

This short survey paper is concerned with a new method to prove global well-posedness results for dispersive equations below energy spaces, namely for the Schrödinger equat…

math.AP2002

Almost conservation laws and global rough solutions to a Nonlinear Schrödinger equation

J. Colliander, M. Keel, G. Staffilani +2

We prove an "almost conservation law" to obtain global-in-time well-posedness for the cubic, defocussing nonlinear Schrödinger equation in H^s(R^n) when n = 2, 3 and s > 4/7, 5/6,…