Lateral earth pressure

In complex network theory, the fitness model is a model of the evolution of a network: how the links between nodes change over time depends on the fitness of nodes. Fitter nodes attract more links at the expense of less fit nodes.

It has been used to model the network structure of the World Wide Web.

Description of the model

The model is based on the idea of fitness, an inherent competitive factor that nodes may have, capable of affecting the network's evolution. According to this idea, the nodes' intrinsic ability to attract links in the network varies from node to node, the most efficient (or "fit") being able to gather more edges in the expense of others. In that sense, not all nodes are identical to each other, and they claim their degree increase according to the fitness they possess every time. The fitness factors of all the nodes composing the network may form a distribution ρ(η) characteristic of the system been studied.

Bianconi and Barabási proposed a new model called Bianconi-Barabasi model, a variant to the Barabási-Albert model (BA model), where the probability for a node to connect to another one is supplied with a term expressing the fitness of the node involved. The fitness parameter is time independent and is multiplicative to the probability

${\mathrm{\Pi }}_i=\frac{{\eta }_i{k}_i}{\sum _j{\eta }_j{k}_j}.$

Thus, the system of equations for the time evolution of the degrees $k_i$ according to the continuum theory introduced by the same model will have the form

$\frac{\partial k_i}{\partial t}=m{\mathrm{\Pi }}_i=m\frac{{\eta }_i{k}_i}{\sum _j{\eta }_j{k}_j}$

where m the number of edges the newly coming node has. If we require the solution to have a similar form to the one it had without the insertion of the fitness factors (to avoid ruining the power-law degree distribution of scale-free networks), then the exponent of the solution has to change and become fitness dependent

$k_{\eta }(t,t_i)=m{\left(\frac{t}{t_i}\right)}^{\beta ({\eta }_i)}$

where

$\beta (\eta )=\frac{\eta }{C}\text{ and }C=\int \rho (\eta )\frac{\eta }{1-\beta (\eta )}d\eta .$

Hence, the more fit nodes increase their degree faster than the less ones. This characteristic attributes the network with a different behavior regarding its evolution. Without the introduction of the fitness property, all nodes had the same exponent in the power-law degree evolution formula. This means that the older nodes in the system would have more edges compared to newcoming ones. After the fitness property is introduced, this exponent, and accordingly, the slope of $k(t)$ change, giving thus the opportunity to newcoming nodes to dominate the system.

It was seen through this example how can a network's evolution change behavior through the introduction of a new parameter in the model. However, we require the network to preserve its overall scale-free character. By forcing the fitness dependence to be accumulated in the exponent only, the degree-distribution will still be a power-law relationship, composed though by a weighted sum of different power-law in degree-evolution formulas

$P(k)\sim \int \rho (\eta )\frac{C}{\eta }(m/k{)}^{C/\eta +1}d\eta$

where ρ(η) is the fitness distribution depending on the system's composition

The fitness model can be extended to in corporate additional processes, such as internal edges, which affect the exponents.

Fitness model and the evolution of the Web

The fitness model has been used to model the network structure of the World Wide Web. In a PNAS article, Kong et al. extended the fitness model to include random node deletion, a common phenomena in the Web. When the deletion rate of the web pages are accounted for, they found that the overall fitness distribution is exponential. Nonetheless, even this small variance in the fitness is amplified through the preferential attachment mechanism, leading to a heavy-tailed distribution of incoming links on the Web.

See also

• Bose–Einstein condensation: a network theory approach