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A Set of Master Variables for the Two-Star Random Graph.

Pawat Akara-Pipattana1, Oleg Evnin2,3

  • 1Université Paris-Saclay, CNRS, LPTMS, 91405 Orsay, France.

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Summary
This summary is machine-generated.

We introduce master variables for large random graphs, simplifying analysis. This method precisely calculates corrections to existing models in dense and sparse graph regimes.

Keywords:
exponential random graph modelslarge N methodsstatistical field theory

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Area of Science:

  • Statistical physics
  • Network science
  • Graph theory

Background:

  • Exponential random graph models are crucial for network analysis.
  • The two-star model is the simplest with edge interactions.
  • Analyzing large networks (N → ∞) requires robust theoretical frameworks.

Purpose of the Study:

  • To develop a novel method for analyzing large exponential random graphs.
  • To introduce auxiliary 'master variables' for controlling the thermodynamic limit.
  • To provide explicit control over 1/N corrections in graph theory.

Main Methods:

  • Introduction of auxiliary 'master variables' to manage the thermodynamic limit (N → ∞).
  • Application of these variables to analyze both dense and sparse graph regimes.
  • Derivation of corrections to the mean-field solution without functional integrals.

Main Results:

  • The method recovers the Park-Newman mean-field solution for dense graphs with explicit 1/N correction control.
  • The first subleading correction to the Park-Newman result is computed, quantifying nonextensive free energy contributions.
  • A compact derivation of the Annibale-Courtney solution for sparse graphs is achieved, bypassing complex functional integral methods.

Conclusions:

  • The proposed 'master variable' approach offers a powerful and simplified framework for large N random graph analysis.
  • This method provides explicit control over corrections, enhancing the accuracy of theoretical predictions.
  • It offers a more accessible alternative to existing techniques for studying sparse and dense random graph models.