Core-halo instability in dynamical systems
Abstract
This paper proves an instability theorem for dynamical systems. As one adds interactions between subystems in a complex system, structured or random, a threshold of connectivity is reached beyond which the overall dynamics inevitably goes unstable. The threshold occurs at the point at which flows and interactions between subsystems (`surface' effects) overwhelm internal stabilizing dynamics (`volume' effects). The theorem is used to identify instability thresholds in systems that possess a core-halo or core-periphery structure, including the gravo-thermal catastrophe -- i.e., star collapse and explosion -- and the interbank payment network. In the core-halo model, the same dynamical instability underlies both gravitational and financial collapse.
Keywords
Cite
@article{arxiv.1302.3199,
title = {Core-halo instability in dynamical systems},
author = {Seth Lloyd},
journal= {arXiv preprint arXiv:1302.3199},
year = {2015}
}
Comments
18 pages, 2 figures, latex