NOLEN-SCHIFFER ANOMALY AND RHO(0)-OMEGA MIXING

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dc.contributor.authorKrein, G.
dc.contributor.institutionUniversidade Estadual Paulista (Unesp)
dc.date.accessioned2014-05-20T15:21:01Z
dc.date.available2014-05-20T15:21:01Z
dc.date.issued1994-12-01
dc.description.abstractThe Nolen-Schiffer anomaly is the long standing discrepancy between theory and experiment of binding energy differences of mirror nuclei. It appears that the anomaly is largely explained by the charge symmetry breaking force generated by the rho(0)-omega mixing. In this paper I discuss the effect of the rho(0)-omega mixing to the binding energy differences in relativistic models of the nucleus. I also discuss the issue of momentum dependence of rho(0)-omega mixing amplitude and present an alternative explanation of the anomaly based on the partial restoration of chiral symmetry in the nucleus.en
dc.description.affiliationUNIV ESTADUAL PAULISTA,INST FIS TEOR,RUA PAMPLONA 145,BR-01405900 SAO PAULO,BRAZIL
dc.description.affiliationUnespUNIV ESTADUAL PAULISTA,INST FIS TEOR,RUA PAMPLONA 145,BR-01405900 SAO PAULO,BRAZIL
dc.format.extent1291-1301
dc.identifierhttp://psroc.phys.ntu.edu.tw/cjp/issues.php
dc.identifier.citationChinese Journal of Physics. Taipei: Physical Soc Republic China, v. 32, n. 6, p. 1291-1301, 1994.
dc.identifier.issn0577-9073
dc.identifier.urihttp://hdl.handle.net/11449/32200
dc.identifier.wosWOS:A1994QV52400033
dc.language.isoeng
dc.publisherPhysical Soc Republic China
dc.relation.ispartofChinese Journal of Physics
dc.relation.ispartofjcr1.051
dc.relation.ispartofsjr0,216
dc.rights.accessRightsAcesso restrito
dc.sourceWeb of Science
dc.titleNOLEN-SCHIFFER ANOMALY AND RHO(0)-OMEGA MIXINGen
dc.typeArtigo
dcterms.licensehttp://psroc.phys.ntu.edu.tw/cjp/author.php
dcterms.rightsHolderPhysical Soc Republic China
unesp.author.orcid0000-0003-1713-8578[1]
unesp.campusUniversidade Estadual Paulista (Unesp), Instituto de Física Teórica (IFT), São Paulopt

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