Stabilization of synchronous tridiagonal network motion
<|reference_start|>Stabilization of synchronous tridiagonal network motion: We consider a network of identical agents, coupled through linear asymmetric coupling. An important case is when each agent has an asymptotically stable periodic orbit, so that the full network inherits a synchronous periodic orbit, but also chaotic trajectories are of interest. In this work, we will restrict to "nearest-neighbor" type of couplings.   The Master Stability Function (MSF) is a powerful tool to establish local stability of the synchronous orbit, in particular a negative MSF implies asymptotic stability. But not every network structure gives a negative MSF. Moreover, there are many situations where in order to obtain a negative MSF, symmetric networks need a coupling strength so large, that the model bears little physical interest. We make two main contributions: (i) Given a tridiagonal nearest neighbor topology, we show how it is possible to choose appropriate coupling so that the synchronous orbit is stable, and (ii) we show that this stability comes without the need of a large coupling strength if the structure is not symmetric. Our construction is based on solving inverse eigenvalue problems. We will see that the coupling of the agents cannot always be chosen to be symmetric so that the underlying graph structure is that of a directed graph with edges having different weights. We provide numerical implementation of our technique on networks of van der Pol and of chaotic R\"ossler oscillators, where the standard symmetric nearest neighbor coupling fails to give stability of the synchronous orbit.<|reference_end|>
@article{dieci2024stabilization,
    title={Stabilization of synchronous tridiagonal network motion},
    author={Luca Dieci, Cinzia Elia, Alessandro Pugliese},
    journal={arXiv preprint arXiv:2408.01066},
    year={2024},
    archivePrefix={arXiv},
    eprint={2408.01066},
    primaryClass={math.DS cs.NA math.NA}
}