# Almost global solutions to two classes of 1-d Hamiltonian Derivative   Nonlinear Schr\"odinger equations

**Authors:** Jing Zhang

arXiv: 1902.06117 · 2019-02-19

## TL;DR

This paper proves almost global existence for two classes of 1-d Hamiltonian Derivative Nonlinear Schr"odinger equations with unbounded nonlinearities, using Birkhoff normal forms and symmetry properties under periodic boundary conditions.

## Contribution

It develops a method to establish long-time solutions for Hamiltonian DNLS equations with unbounded nonlinearities by constructing Birkhoff normal forms and exploiting symmetry.

## Key findings

- Solutions remain small over long time intervals proportional to \\varepsilon^{-r_*}
- Most potentials lead to almost global solutions for small initial data
- Method handles unbounded nonlinearities in Hamiltonian systems

## Abstract

Consider two kinds of 1-d Hamiltonian Derivative Nonlinear Schr\"odinger (DNLS) equations with respect to different symplectic forms under periodic boundary conditions. The nonlinearities of these equations depend not only on $(x,\psi,\bar{\psi})$ but also on $(\psi_x,\bar{\psi}_x)$, which means the nonlinearities of these equations are unbounded. Suppose that the nonlinearities depend on the space-variable $x$ periodically.   Under some assumptions, for most potentials of these two kinds of Hamiltonian DNLS equations, if the initial value is smaller than $\varepsilon\ll1$ in $p$-Sobolev norm, then the corresponding solution to these equations is also smaller than $2\varepsilon$ during a time interval $(-c\varepsilon^{-r_*},c\varepsilon^{-r_*})$(for any given positive $r_*$). The main methods are constructing Birkhoff normal forms to two kinds of Hamiltonian systems which have unbounded nonlinearities and using the special symmetry of the unbounded nonlinearities of Hamiltonian functions to obtain a long time estimate of the solution in $p$-Sobolev norm.

## Full text

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## References

39 references — full list in the complete paper: https://tomesphere.com/paper/1902.06117/full.md

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Source: https://tomesphere.com/paper/1902.06117