Continuum dynamics of the intention field under weakly cohesive social interaction
We investigate the long-time dynamics of an opinion formation model inspired by a work by Borghesi, Bouchaud and Jensen. First, we derive a Fokker–Planck-type equation under the assumption that interactions between individuals produce little consensus of opinion (grazing collision approximation). Se...
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| Published in | Mathematical models & methods in applied sciences Vol. 27; no. 1; pp. 159 - 182 |
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| Main Authors | , , , |
| Format | Journal Article |
| Language | English |
| Published |
Singapore
World Scientific Publishing Company
01.01.2017
World Scientific Publishing Co. Pte., Ltd World Scientific Publishing |
| Subjects | |
| Online Access | Get full text |
| ISSN | 0218-2025 1793-4060 1793-6314 1793-6314 |
| DOI | 10.1142/S021820251740005X |
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| Summary: | We investigate the long-time dynamics of an opinion formation model inspired by a work by Borghesi, Bouchaud and Jensen. First, we derive a Fokker–Planck-type equation under the assumption that interactions between individuals produce little consensus of opinion (grazing collision approximation). Second, we study conditions under which the Fokker–Planck equation has non-trivial equilibria and derive the macroscopic limit (corresponding to the long-time dynamics and spatially localized interactions) for the evolution of the mean opinion. Finally, we compare two different types of interaction rates: the original one given in the work of Borghesi, Bouchaud and Jensen (symmetric binary interactions) and one inspired from works by Motsch and Tadmor (non-symmetric binary interactions). We show that the first case leads to a conservative model for the density of the mean opinion whereas the second case leads to a non-conservative equation. We also show that the speed at which consensus is reached asymptotically for these two rates has fairly different density dependence. |
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| Bibliography: | ObjectType-Article-1 SourceType-Scholarly Journals-1 ObjectType-Feature-2 content type line 14 |
| ISSN: | 0218-2025 1793-4060 1793-6314 1793-6314 |
| DOI: | 10.1142/S021820251740005X |