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This paper presents a novel mathematical framework for analyzing sparse graphs by mapping them to their dense line graphs, thereby enabling the estimation of graph limits (graphons) that would otherwise vanish due to sparsity. By leveraging this transformation, researchers can distinguish between different types of sparse network structures, such as star graphs and preferential attachment models, using established tools from dense graph theory. The work advances theoretical machine learning by providing a rigorous method to infer underlying distributional properties from limited observational data in combinatorial settings.
Graphons of Line Graphs
arXiv:2409.01656v4 Announce Type: replace-cross Abstract: We consider the problem of estimating graph limits, known as graphons, from observations of sequences of sparse finite graphs. In this paper we show a simple method that can shed light on a subset of sparse graphs. The method involves mapping the original graphs to their line graphs. We show that graphs satisfying a particular property, which we call the square-degree property are sparse, but give rise to dense line graphs. This enables the use of results on graph limits of dense graphs to derive convergence. In particular, star graphs satisfy the square-degree property resulting in dense line graphs and non-zero graphons of line graphs. We demonstrate empirically that we can distinguish different numbers of stars (which are sparse) by the graphons of their corresponding line graphs. Whereas in the original graphs, the different number of stars all converge to the zero graphon due to sparsity. Similarly, superlinear preferential attachment graphs give rise to dense line graphs almost surely. In contrast, dense graphs, including Erdos-Renyi graphs make the line graphs sparse, resulting in the zero graphon.
Abstract:We consider the problem of estimating graph limits, known as graphons, from observations of sequences of sparse finite graphs. In this paper we show a simple method that can shed light on a subset of sparse graphs. The method involves mapping the original graphs to their line graphs. We show that graphs satisfying a particular property, which we call the square-degree property are sparse, but give rise to dense line graphs. This enables the use of results on graph limits of dense graphs to derive convergence. In particular, star graphs satisfy the square-degree property resulting in dense line graphs and non-zero graphons of line graphs. We demonstrate empirically that we can distinguish different numbers of stars (which are sparse) by the graphons of their corresponding line graphs. Whereas in the original graphs, the different number of stars all converge to the zero graphon due to sparsity. Similarly, superlinear preferential attachment graphs give rise to dense line graphs almost surely. In contrast, dense graphs, including Erdos-Renyi graphs make the line graphs sparse, resulting in the zero graphon.
Machine Learning (stat.ML); Discrete Mathematics (cs.DM); Machine Learning (cs.LG); Combinatorics (math.CO)
arXiv:2409.01656 [stat.ML]
(or arXiv:2409.01656v4 [stat.ML] for this version)
https://doi.org/10.48550/arXiv.2409.01656 Focus to learn more arXiv-issued DOI via DataCite
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