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Please use this identifier to cite or link to this item: http://acervodigital.unesp.br/handle/11449/23941
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dc.contributor.authorAnanos, G. N. J.-
dc.date.accessioned2014-05-20T14:08:14Z-
dc.date.accessioned2016-10-25T17:14:09Z-
dc.date.available2014-05-20T14:08:14Z-
dc.date.available2016-10-25T17:14:09Z-
dc.date.issued2004-01-01-
dc.identifierhttp://dx.doi.org/10.1063/1.1843688-
dc.identifier.citationIx Hadron Physics and Vii Relativistic Aspects of Nuclear Physics. Melville: Amer Inst Physics, v. 739, p. 672-674, 2004.-
dc.identifier.issn0094-243X-
dc.identifier.urihttp://hdl.handle.net/11449/23941-
dc.identifier.urihttp://acervodigital.unesp.br/handle/11449/23941-
dc.description.abstractWe discuss the phi(6) theory defined in D = 2 + 1-dimensional space-time and assume that the system is in equilibrium with a thermal bath at temperature beta(-1). We use the 1/N expansion and the method of composite operator (CJT) for summing a large set of Feynman graphs. We demonstrate explicitly the Coleman-Mermin-Wagner theorem at finite temperature.en
dc.format.extent672-674-
dc.language.isoeng-
dc.publisherAmerican Institute of Physics (AIP)-
dc.sourceWeb of Science-
dc.titleScalar field theory at finite temperature in D=2+1en
dc.typeoutro-
dc.contributor.institutionUniversidade Estadual Paulista (UNESP)-
dc.description.affiliationUniv Estadual Paulista, Inst Fis Teor, BR-01405900 São Paulo, Brazil-
dc.description.affiliationUnespUniv Estadual Paulista, Inst Fis Teor, BR-01405900 São Paulo, Brazil-
dc.identifier.doi10.1063/1.1843688-
dc.identifier.wosWOS:000226476000098-
dc.rights.accessRightsAcesso restrito-
dc.relation.ispartofIx Hadron Physics and Vii Relativistic Aspects of Nuclear Physics-
Appears in Collections:Artigos, TCCs, Teses e Dissertações da Unesp

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