A duplex voter model on multiplex networks exhibits spontaneous symmetry-breaking and a cusp bifurcation with noise that unfolds explosive versus non-explosive transitions.
Multilayer network science: theory, methods, and applications
2 Pith papers cite this work. Polarity classification is still indexing.
abstract
Multilayer network science has emerged as a central framework for analysing interconnected and interdependent complex systems. Its relevance has grown substantially with the increasing availability of rich, heterogeneous data, which makes it possible to uncover and exploit the inherently multilayered organisation of many real-world networks. In this review, we summarise recent developments in the field. On the theoretical and methodological front, we outline core concepts and survey advances in community detection, dynamical processes, temporal networks, higher-order interactions, and machine-learning-based approaches. On the application side, we discuss progress across diverse domains, including interdependent infrastructures, spreading dynamics, computational social science, economic and financial systems, ecological and climate networks, science-of-science studies, network medicine, and network neuroscience. We conclude with a forward-looking perspective, emphasizing the need for standardised datasets and software, deeper integration of temporal and higher-order structures, and a transition toward genuinely predictive models of complex systems.
years
2026 2verdicts
UNVERDICTED 2representative citing papers
Epidemic models on multigraphs and simple graphs with identical degree sequences differ only when activity persists exponentially long on star-like hubs.
citing papers explorer
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Symmetry-Breaking and Hysteresis in a Duplex Voter Model
A duplex voter model on multiplex networks exhibits spontaneous symmetry-breaking and a cusp bifurcation with noise that unfolds explosive versus non-explosive transitions.
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Epidemic spreading on multigraphs
Epidemic models on multigraphs and simple graphs with identical degree sequences differ only when activity persists exponentially long on star-like hubs.