dc.contributorTEL AVIV UNIV
dc.contributorUniversidade Estadual Paulista (Unesp)
dc.contributorUniversidade de São Paulo (USP)
dc.date.accessioned2014-05-20T15:26:59Z
dc.date.accessioned2022-10-05T16:40:38Z
dc.date.available2014-05-20T15:26:59Z
dc.date.available2022-10-05T16:40:38Z
dc.date.created2014-05-20T15:26:59Z
dc.date.issued1996-07-25
dc.identifierPhysics Letters B. Amsterdam: Elsevier B.V., v. 381, n. 4, p. 385-390, 1996.
dc.identifier0370-2693
dc.identifierhttp://hdl.handle.net/11449/37050
dc.identifier10.1016/0370-2693(96)00591-6
dc.identifierWOS:A1996UZ00200002
dc.identifier.urihttp://repositorioslatinoamericanos.uchile.cl/handle/2250/3908644
dc.description.abstractBinding energy differences of mirror nuclei for A = 15, 17, 27, 29, 31, 33, 39 and 41 are calculated in the framework of relativistic deformed mean-field theory. To fully include the effects of the polarization of the nuclear core due to the extra particle or hole, the spatial components of the vector meson fields and the photon are taken into account in a self-consistent manner. The calculated binding energy differences are systematically smaller than the experimental values and lend support to the existency of the Okamoto-Nolen-Schiffer anomaly found decades ago in nonrelativistic calculations, For the majority of the nuclei studied, however, the results are such that the anomaly is significantly smaller than the one obtained within state-of-the-art nonrelativistic calculations.
dc.languageeng
dc.publisherElsevier B.V.
dc.relationPhysics Letters B
dc.relation4.254
dc.relation2,336
dc.rightsAcesso restrito
dc.sourceWeb of Science
dc.titleRelativistic deformed mean-field calculation of binding energy differences of mirror nuclei
dc.typeArtigo


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