# Asymptotic stability of robust heteroclinic networks

**Authors:** Olga Podvigina, Sofia B.S.D. Castro, Isabel S. Labouriau

arXiv: 1905.06419 · 2020-04-22

## TL;DR

This paper establishes conditions under which certain robust heteroclinic networks, specifically ac-networks in symmetric dynamical systems, are asymptotically stable, with proofs and applications to examples.

## Contribution

It provides new sufficient conditions for the asymptotic stability of ac-networks in symmetric systems, expanding understanding of heteroclinic network stability.

## Key findings

- Sufficient conditions for stability of ac-networks
- Classification of ac-networks via graph types
- Application to specific heteroclinic network examples

## Abstract

We provide conditions guaranteeing that certain classes of robust heteroclinic networks are asymptotically stable.   We study the asymptotic stability of ac-networks --- robust heteroclinic networks that exist in smooth ${\mathbb Z}^n_2$-equivariant dynamical systems defined in the positive orthant of ${\mathbb R}^n$. Generators of the group ${\mathbb Z}^n_2$ are the transformations that change the sign of one of the spatial coordinates. The ac-network is a union of hyperbolic equilibria and connecting trajectories, where all equilibria belong to the coordinate axes (not more than one equilibrium per axis) with unstable manifolds of dimension one or two. The classification of ac-networks is carried out by describing all possible types of associated graphs.   We prove sufficient conditions for asymptotic stability of ac-networks. The proof is given as a series of theorems and lemmas that are applicable to the ac-networks and to more general types of networks. Finally, we apply these results to discuss the asymptotic stability of several examples of heteroclinic networks.

## Full text

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## Figures

27 figures with captions in the complete paper: https://tomesphere.com/paper/1905.06419/full.md

## References

34 references — full list in the complete paper: https://tomesphere.com/paper/1905.06419/full.md

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Source: https://tomesphere.com/paper/1905.06419