Coexistence of interacting opinions in a generalized Sznajd model

André M. Timpanaro and Carmen P. C. Prado
Phys. Rev. E 84, 027101 – Published 4 August 2011

Abstract

The Sznajd model is a sociophysics model that mimics the propagation of opinions in a closed society, where the interactions favor groups of agreeing people. It is based in the Ising and Potts ferromagnetic models and, although the original model used only linear chains, it has since been adapted to general networks. This model has a very rich transient, which has been used to model several aspects of elections, but its stationary states are always consensus states. In order to model more complex behaviors, we have, in a recent work, introduced the idea of biases and prejudices to the Sznajd model by generalizing the bounded confidence rule, which is common to many continuous opinion models, to what we called confidence rules. In that work we have found that the mean field version of this model (corresponding to a complete network) allows for stationary states where noninteracting opinions survive, but never for the coexistence of interacting opinions. In the present work, we provide networks that allow for the coexistence of interacting opinions for certain confidence rules. Moreover, we show that the model does not become inactive; that is, the opinions keep changing, even in the stationary regime. This is an important result in the context of understanding how a rule that breeds local conformity is still able to sustain global diversity while avoiding a frozen stationary state. We also provide results that give some insights on how this behavior approaches the mean field behavior as the networks are changed.

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  • Received 30 March 2011

DOI:https://doi.org/10.1103/PhysRevE.84.027101

©2011 American Physical Society

Authors & Affiliations

André M. Timpanaro* and Carmen P. C. Prado

  • Instituto de Física, Universidade de São Paulo, Caixa Postal 66318, 05314-970 São Paulo, São Paulo, Brazil

  • *timpa@if.usp.br
  • prado@if.usp.br

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Vol. 84, Iss. 2 — August 2011

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