4.7 Article

Analytic solution of the two-star model with correlated degrees

期刊

PHYSICAL REVIEW E
卷 104, 期 1, 页码 -

出版社

AMER PHYSICAL SOC
DOI: 10.1103/PhysRevE.104.014147

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  1. CAPES/Brazil
  2. London Mathematical Laboratory
  3. CNPq/Brazil

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The study investigates the characteristics of the two-star model with degree-degree correlations in the sparse regime, revealing a first-order transition to a condensed phase and different degree distribution features based on different degree correlations. The research also finds that degree assortativities are nonmonotonic functions of the model parameters, exhibiting discontinuous behavior.
Exponential random graphs are important to model the structure of real-world complex networks. Here we solve the two-star model with degree-degree correlations in the sparse regime. The model constraints the average correlation between the degrees of adjacent nodes (nearest neighbors) and between the degrees at the end-points of two-stars (next nearest neighbors). We compute exactly the network free energy and show that this model undergoes a first-order transition to a condensed phase. For non-negative degree correlations between next nearest neighbors, the degree distribution inside the condensed phase has a single peak at the largest degree, while for negative degree correlations between next nearest neighbors the condensed phase is characterized by a bimodal degree distribution. We calculate the degree assortativities and show they are nonmonotonic functions of the model parameters, with a discontinuous behavior at the first-order transition. The first-order critical line terminates at a second-order critical point, whose location in the phase diagram can be accurately determined. Our results can help to develop more detailed models of complex networks with correlated degrees.

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