Abstract

Preferential attachment --- by which new nodes attach to existing nodes with probability proportional to the existing nodes' degree --- has become the standard growth model for scale-free networks, where the asymptotic probability of a node having degree kk is proportional to k−γk^{-γ}. However, the motivation for this model is entirely ad hoc. We use exact likelihood arguments and show that the optimal way to build a scale-free network is to attach most new links to nodes of low degree. Curiously, this leads to a scale-free networks with a single dominant hub: a star-like structure we call a super-star network. Asymptotically, the optimal strategy is to attach each new node to one of the nodes of degree kk with probability proportional to 1N+ζ(γ)(k+1)γ\frac{1}{N+ζ(γ)(k+1)^γ} (in a NN node network) --- a stronger bias toward high degree nodes than exhibited by standard preferential attachment. Our algorithm generates optimally scale-free networks (the super-star networks) as well as randomly sampling the space of all scale-free networks with a given degree exponent γγ. We generate viable realisation with finite NN for 1≪γ<21\ll γ<2 as well as γ>2γ>2. We observe an apparently discontinuous transition at γ≈2γ\approx 2 between so-called super-star networks and more tree-like realisations. Gradually increasing γγ further leads to re-emergence of a super-star hub. To quantify these structural features we derive a new analytic expression for the expected degree exponent of a pure preferential attachment process, and introduce alternative measures of network entropy. Our approach is generic and may also be applied to an arbitrary degree distribution.

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