DC Field | Value | Language |
---|---|---|
dc.contributor.author | Park, J | ko |
dc.contributor.author | Newman, MEJ | ko |
dc.date.accessioned | 2013-03-06T04:58:37Z | - |
dc.date.available | 2013-03-06T04:58:37Z | - |
dc.date.created | 2012-10-18 | - |
dc.date.created | 2012-10-18 | - |
dc.date.created | 2012-10-18 | - |
dc.date.issued | 2004-12 | - |
dc.identifier.citation | PHYSICAL REVIEW E, v.70, no.6 | - |
dc.identifier.issn | 1539-3755 | - |
dc.identifier.uri | http://hdl.handle.net/10203/85873 | - |
dc.description.abstract | The p-star model or exponential random graph is among the oldest and best known of network models. Here we give an analytic solution for the particular case of the two-star model, which is one of the most fundamental of exponential random graphs. We derive expressions for a number of quantities of interest in the model and show that the degenerate region of the parameter space observed in computer simulations is a spontaneously symmetry-broken phase separated from the normal phase of the model by a conventional continuous phase transition. | - |
dc.language | English | - |
dc.publisher | AMER PHYSICAL SOC | - |
dc.title | Solution of the two-star model of a network | - |
dc.type | Article | - |
dc.identifier.wosid | 000226299200053 | - |
dc.identifier.scopusid | 2-s2.0-37649029297 | - |
dc.type.rims | ART | - |
dc.citation.volume | 70 | - |
dc.citation.issue | 6 | - |
dc.citation.publicationname | PHYSICAL REVIEW E | - |
dc.identifier.doi | 10.1103/PhysRevE.70.066146 | - |
dc.contributor.localauthor | Park, J | - |
dc.contributor.nonIdAuthor | Newman, MEJ | - |
dc.type.journalArticle | Article | - |
dc.subject.keywordPlus | COMPLEX NETWORKS | - |
dc.subject.keywordPlus | SOCIAL NETWORKS | - |
dc.subject.keywordPlus | MARKOV GRAPHS | - |
dc.subject.keywordPlus | LOGIT-MODELS | - |
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