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Article: Network compression with configuration models and the minimum description length

TitleNetwork compression with configuration models and the minimum description length
Authors
Issue Date6-Sep-2024
PublisherAmerican Physical Society
Citation
Physical Review E, 2024, v. 110, n. 3 How to Cite?
Abstract

Random network models, constrained to reproduce specific statistical features, are often used to represent and analyze network data and their mathematical descriptions. Chief among them, the configuration model constrains random networks by their degree distribution and is foundational to many areas of network science. However, configuration models and their variants are often selected based on intuition or mathematical and computational simplicity rather than on statistical evidence. To evaluate the quality of a network representation, we need to consider both the amount of information required to specify a random network model and the probability of recovering the original data when using the model as a generative process. To this end, we calculate the approximate size of network ensembles generated by the popular configuration model and its generalizations, including versions accounting for degree correlations and centrality layers. We then apply the minimum description length principle as a model selection criterion over the resulting nested family of configuration models. Using a dataset of over 100 networks from various domains, we find that the classic configuration model is generally preferred on networks with an average degree above 10, while a layered configuration model constrained by a centrality metric offers the most compact representation of the majority of sparse networks.


Persistent Identifierhttp://hdl.handle.net/10722/362877
ISSN
2023 Impact Factor: 2.2
2023 SCImago Journal Rankings: 0.805

 

DC FieldValueLanguage
dc.contributor.authorHébert-Dufresne, Laurent-
dc.contributor.authorYoung, Jean Gabriel-
dc.contributor.authorDaniels, Alexander-
dc.contributor.authorKirkley, Alec-
dc.contributor.authorAllard, Antoine-
dc.date.accessioned2025-10-03T00:35:45Z-
dc.date.available2025-10-03T00:35:45Z-
dc.date.issued2024-09-06-
dc.identifier.citationPhysical Review E, 2024, v. 110, n. 3-
dc.identifier.issn2470-0045-
dc.identifier.urihttp://hdl.handle.net/10722/362877-
dc.description.abstract<p>Random network models, constrained to reproduce specific statistical features, are often used to represent and analyze network data and their mathematical descriptions. Chief among them, the configuration model constrains random networks by their degree distribution and is foundational to many areas of network science. However, configuration models and their variants are often selected based on intuition or mathematical and computational simplicity rather than on statistical evidence. To evaluate the quality of a network representation, we need to consider both the amount of information required to specify a random network model and the probability of recovering the original data when using the model as a generative process. To this end, we calculate the approximate size of network ensembles generated by the popular configuration model and its generalizations, including versions accounting for degree correlations and centrality layers. We then apply the minimum description length principle as a model selection criterion over the resulting nested family of configuration models. Using a dataset of over 100 networks from various domains, we find that the classic configuration model is generally preferred on networks with an average degree above 10, while a layered configuration model constrained by a centrality metric offers the most compact representation of the majority of sparse networks.</p>-
dc.languageeng-
dc.publisherAmerican Physical Society-
dc.relation.ispartofPhysical Review E-
dc.rightsThis work is licensed under a Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License.-
dc.titleNetwork compression with configuration models and the minimum description length-
dc.typeArticle-
dc.identifier.doi10.1103/PhysRevE.110.034305-
dc.identifier.scopuseid_2-s2.0-85203599285-
dc.identifier.volume110-
dc.identifier.issue3-
dc.identifier.eissn2470-0053-
dc.identifier.issnl2470-0045-

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