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Please use this identifier to cite or link to this item: http://acervodigital.unesp.br/handle/11449/130694
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dc.contributor.authorAbdalla, E.-
dc.contributor.authorAbdalla, M. C B-
dc.contributor.authorDevecchi, F. P.-
dc.contributor.authorZadra, A.-
dc.date.accessioned2014-05-27T05:18:59Z-
dc.date.accessioned2016-10-25T21:21:48Z-
dc.date.available2014-05-27T05:18:59Z-
dc.date.available2016-10-25T21:21:48Z-
dc.date.issued1988-12-22-
dc.identifierhttp://dx.doi.org/10.1016/0370-2693(88)91360-3-
dc.identifier.citationPhysics Letters B, v. 215, n. 3, p. 564-566, 1988.-
dc.identifier.issn0370-2693-
dc.identifier.urihttp://hdl.handle.net/11449/130694-
dc.identifier.urihttp://acervodigital.unesp.br/handle/11449/130694-
dc.description.abstractStarting out with an anomaly free lagrangian formulation for chiral scalars, which includes a Wess-Zumino term (to cancel the anomaly), we formulate the corresponding hamiltonian problem. Then we use the (quantum) Siegel invariance to choose a particular solution, which turns out to coincide with the one obtained by Floreanini and Jackiw. © 1988.en
dc.format.extent564-566-
dc.language.isoeng-
dc.publisherElsevier B.V.-
dc.sourceScopus-
dc.titleHamiltonian formulation of anomaly free chiral bosonsen
dc.typeoutro-
dc.contributor.institutionUniversidade de São Paulo (USP)-
dc.contributor.institutionUniversidade Estadual Paulista (UNESP)-
dc.description.affiliationInstituto de Fisica Universidade de Sao Paulo, CP 20516, 01498 Sao Paulo-
dc.description.affiliationInstituto de Fisica Teorica Universidade Estadual Paulista, Rua Pamplona 145, 01408 Sao Paulo-
dc.description.affiliationUnespInstituto de Fisica Teorica Universidade Estadual Paulista, Rua Pamplona 145, 01408 Sao Paulo-
dc.identifier.doi10.1016/0370-2693(88)91360-3-
dc.identifier.wosWOS:A1988R576800025-
dc.rights.accessRightsAcesso restrito-
dc.relation.ispartofPhysics Letters B-
dc.identifier.scopus2-s2.0-45449123474-
Appears in Collections:Artigos, TCCs, Teses e Dissertações da Unesp

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