Colorful Star Motif Counting: Concepts, Algorithms and Applications

A colorful star motif is a star-shaped graph where any two nodes have different colors. Counting the colorful star motif can help to analyze the structural properties of real-life colorful graphs, model higher-order clustering, and accelerate the mining of the densest subgraph exhibiting <inline-formula><tex-math notation="LaTeX">$h$</tex-math></inline-formula>-clique characteristics in graphs. In this manuscript, we introduce the concept of colorful <inline-formula><tex-math notation="LaTeX">$h$</tex-math></inline-formula>-star in a colored graph and proposes two higher-order cohesive subgraph models, namely colorful <inline-formula><tex-math notation="LaTeX">$h$</tex-math></inline-formula>-star core and colorful <inline-formula><tex-math notation="LaTeX">$h$</tex-math></inline-formula>-star truss. We show that the colorful <inline-formula><tex-math notation="LaTeX">$h$</tex-math></inline-formula>-stars can be counted and updated very efficiently using a novel dynamic programming (DP) algorithm. Based on the proposed DP algorithm, we develop a colorful <inline-formula><tex-math notation="LaTeX">$h$</tex-math></inline-formula>-star core decomposition algorithm which takes <inline-formula><tex-math notation="LaTeX">$O(h m)$</tex-math></inline-formula> time, <inline-formula><tex-math notation="LaTeX">$O(h n+m)$</tex-math></inline-formula> space; and a colorful <inline-formula><tex-math notation="LaTeX">$h$</tex-math></inline-formula>-star truss decomposition algorithm which takes <inline-formula><tex-math notation="LaTeX">$O(h m^{1.5})$</tex-math></inline-formula> time, <inline-formula><tex-math notation="LaTeX">$O(hm)$</tex-math></inline-formula> space, where <inline-formula><tex-math notation="LaTeX">$m$</tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX">$n$</tex-math></inline-formula> denote the number of edges and nodes of the graph respectively. Moreover, we also propose a graph reduction technique based on our colorful <inline-formula><tex-math notation="LaTeX">$h$</tex-math></inline-formula>-star core model to accelerate the computation of the approximation algorithm for <inline-formula><tex-math notation="LaTeX">$ h$</tex-math></inline-formula>-clique densest subgraph mining. The results of comprehensive experiments on 11 large real-world datasets demonstrate the efficiency, scalability and effectiveness of the proposed algorithms.

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Publication Details

Journal
IEEE Transactions on Knowledge and Data Engineering
Published
2024-12-13
DOI
https://doi.org/10.1109/tkde.2024.3514997
Primary Topic
Astronomical Observations and Instrumentation
Type
article
Field-Weighted Citation Impact
0.00
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article

Colorful Star Motif Counting: Concepts, Algorithms and Applications

Ye Yuan, Hongchao Qin, Yuanyuan Li, Hongzhi Chen et al.
IEEE Transactions on Knowledge and Data Engineering
Astronomical Observations and Instrumentation
article

Colorful Star Motif Counting: Concepts, Algorithms and Applications

Ye Yuan, Hongchao Qin, Yuanyuan Li, Hongzhi Chen, Sen Gao, Guoren Wang
article en

Abstract

A colorful star motif is a star-shaped graph where any two nodes have different colors. Counting the colorful star motif can help to analyze the structural properties of real-life colorful graphs, model higher-order clustering, and accelerate the mining of the densest subgraph exhibiting <inline-formula><tex-math notation="LaTeX">$h$</tex-math></inline-formula>-clique characteristics in graphs. In this manuscript, we introduce the concept of colorful <inline-formula><tex-math notation="LaTeX">$h$</tex-math></inline-formula>-star in a colored graph and proposes two higher-order cohesive subgraph models, namely colorful <inline-formula><tex-math notation="LaTeX">$h$</tex-math></inline-formula>-star core and colorful <inline-formula><tex-math notation="LaTeX">$h$</tex-math></inline-formula>-star truss. We show that the colorful <inline-formula><tex-math notation="LaTeX">$h$</tex-math></inline-formula>-stars can be counted and updated very efficiently using a novel dynamic programming (DP) algorithm. Based on the proposed DP algorithm, we develop a colorful <inline-formula><tex-math notation="LaTeX">$h$</tex-math></inline-formula>-star core decomposition algorithm which takes <inline-formula><tex-math notation="LaTeX">$O(h m)$</tex-math></inline-formula> time, <inline-formula><tex-math notation="LaTeX">$O(h n+m)$</tex-math></inline-formula> space; and a colorful <inline-formula><tex-math notation="LaTeX">$h$</tex-math></inline-formula>-star truss decomposition algorithm which takes <inline-formula><tex-math notation="LaTeX">$O(h m^{1.5})$</tex-math></inline-formula> time, <inline-formula><tex-math notation="LaTeX">$O(hm)$</tex-math></inline-formula> space, where <inline-formula><tex-math notation="LaTeX">$m$</tex-math></inline-formula> and <inline-formula><tex-math notation="LaTeX">$n$</tex-math></inline-formula> denote the number of edges and nodes of the graph respectively. Moreover, we also propose a graph reduction technique based on our colorful <inline-formula><tex-math notation="LaTeX">$h$</tex-math></inline-formula>-star core model to accelerate the computation of the approximation algorithm for <inline-formula><tex-math notation="LaTeX">$ h$</tex-math></inline-formula>-clique densest subgraph mining. The results of comprehensive experiments on 11 large real-world datasets demonstrate the efficiency, scalability and effectiveness of the proposed algorithms.

IEEE Transactions on Knowledge and Data EngineeringVol. 37(3)
Beijing Institute of Technology (CN), National University of Singapore (SG)
Openalex Percentile: Top 75%
Astronomical Observations and Instrumentation
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