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Please use this identifier to cite or link to this item: http://acervodigital.unesp.br/handle/11449/67655
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dc.contributor.authorDe Melo, J. P B C-
dc.contributor.authorFrederico, T.-
dc.contributor.authorPace, E.-
dc.contributor.authorSalmè, G.-
dc.date.accessioned2014-05-27T11:21:02Z-
dc.date.accessioned2016-10-25T18:19:24Z-
dc.date.available2014-05-27T11:21:02Z-
dc.date.available2016-10-25T18:19:24Z-
dc.date.issued2004-02-12-
dc.identifierhttp://dx.doi.org/10.1016/j.physletb.2003.11.072-
dc.identifier.citationPhysics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics, v. 581, n. 1-2, p. 75-81, 2004.-
dc.identifier.issn0370-2693-
dc.identifier.urihttp://hdl.handle.net/11449/67655-
dc.identifier.urihttp://acervodigital.unesp.br/handle/11449/67655-
dc.description.abstractThe pion electromagnetic form factor is calculated in the space- and time-like regions from -10 (GeV/c)2 up to 10 (GeV/c)2, within a front-form model. The dressed photon vertex where a photon decays in a quark-antiquark pair is depicted generalizing the vector meson dominance ansatz, by means of the vector meson vertex functions. An important feature of our model is the description of the on-mass-shell vertex functions in the valence sector, for the pion and the vector mesons, through the front-form wave functions obtained within a realistic quark model. The theoretical results show an excellent agreement with the data in the space-like region, while in the time-like region the description is quite encouraging. © 2003 Elsevier B.V. All rights reserved.en
dc.format.extent75-81-
dc.language.isoeng-
dc.sourceScopus-
dc.subjectElectromagnetic form factors-
dc.subjectPion-
dc.subjectRelativistic quark model-
dc.subjectVector-meson dominance-
dc.subjectcalculation-
dc.subjectelectromagnetic field-
dc.subjectmolecular dynamics-
dc.subjectmolecular model-
dc.subjectphoton-
dc.subjectpion-
dc.subjectspace-
dc.subjecttime-
dc.subjectwaveform-
dc.titleElectromagnetic form factor of the pion in the space- and time-like regions within the front-form dynamicsen
dc.typeoutro-
dc.contributor.institutionUniversidade Estadual Paulista (UNESP)-
dc.contributor.institutionCentro Técnico Aeroespacial-
dc.contributor.institutionSezione Tor Vergata-
dc.contributor.institutionSezione Roma I-
dc.description.affiliationInst. de Fís. Teórica Universidade Estadual Paulista, 01405-900 São Paulo, SP-
dc.description.affiliationDepartamento de Física Inst. Tecn. da Aeronáutica Centro Técnico Aeroespacial, 12.228-900 Sao Jose dos Campos, SP-
dc.description.affiliationDipartimento di Fisica Univ. di Roma Tor Vergata Sezione Tor Vergata, Via della Ricerca Scientifica 1, I-00133 Roma-
dc.description.affiliationIst. Nazionale di Fisica Nucleare Sezione Roma I, P.le A. Moro 2, I-00185 Roma-
dc.description.affiliationUnespInst. de Fís. Teórica Universidade Estadual Paulista, 01405-900 São Paulo, SP-
dc.identifier.doi10.1016/j.physletb.2003.11.072-
dc.identifier.wosWOS:000188698200009-
dc.rights.accessRightsAcesso aberto-
dc.identifier.file2-s2.0-1642431873.pdf-
dc.relation.ispartofPhysics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics-
dc.identifier.scopus2-s2.0-1642431873-
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