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Growing Cayley trees described by a Fermi distribution
1Department of Physics, University of Notre Dame, Indiana 46556, USA.
Summary
Thermal noise in growing Cayley trees leads to bond strength distributions following Fermi statistics. Network evolution mirrors Eden and invasion percolation models at different temperature limits.
Area of Science:
- Complex Networks
- Statistical Physics
- Network Science
Background:
- Growing Cayley trees are a model for hierarchical network structures.
- Thermal noise introduces randomness and influences network properties.
- Understanding bond strength distributions is crucial for network behavior.
Purpose of the Study:
- To investigate the statistical properties of bond strengths in growing Cayley trees under thermal noise.
- To determine the applicable statistical mechanics models for network evolution.
- To relate findings to existing network models like scale-free networks.
Main Methods:
- Simulating growing Cayley trees with thermal noise.
- Analyzing the distribution of bond strengths (energies).
- Examining network evolution in limiting temperature cases (T→0 and T→∞).
Main Results:
- The distribution of bond strengths follows Fermi statistics.
- Network evolution converges to the Eden model as temperature approaches zero.
- Network evolution converges to the invasion percolation model as temperature approaches infinity.
Conclusions:
- Fermi statistics accurately describe bond strengths in these growing hierarchical networks.
- The study connects Cayley tree evolution to established models like Eden and invasion percolation.
- Results offer insights into the relationship between network structure and statistical mechanics, including scale-free networks described by Bose statistics.
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