# Time-like boundary conditions in the NLS model

**Authors:** Anastasia Doikou, Iain Findlay, Spyridoula Sklaveniti

arXiv: 1902.07551 · 2019-03-11

## TL;DR

This paper extends the concept of space-time dualities in the integrable non-linear Schrödinger model by introducing and analyzing time-like boundary conditions, conserved quantities, and Lax pairs, including a novel time-like dressing method.

## Contribution

It introduces the first-time development of time-like dressing for the NLS model and identifies boundary conditions via solutions of the reflection equation, expanding integrability understanding.

## Key findings

- Derived the generating function for Lax pair components at time-like boundaries.
- Established analytical conditions for boundary Lax pairs leading to specific boundary conditions.
- Formulated time Riccati equations and conserved quantities for the NLS hierarchy.

## Abstract

We focus on the non-linear Schrodinger model and we extend the notion of space-time dualities in the presence of integrable time-like boundary conditions. We identify the associated time-like `conserved' quantities and Lax pairs as well as the corresponding boundary conditions. In particular, we derive the generating function of the space components of the Lax pairs in the case of time-like boundaries defined by solutions of the reflection equation. Analytical conditions on the boundary Lax pair lead to the time like-boundary conditions. The time-like dressing is also performed for the first time, as an effective means to produce the space components of the Lax pair of the associated hierarchy. This is particularly relevant in the absence of a classical r-matrix, or when considering complicated underlying algebraic structures. The associated time Riccati equations and hence the time-like conserved quantities are also derived. We use as the main paradigm for this purpose the matrix NLS-type hierarchy.

## Full text

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## References

24 references — full list in the complete paper: https://tomesphere.com/paper/1902.07551/full.md

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Source: https://tomesphere.com/paper/1902.07551