dc.contributorInstituto Tecnológico de Aeronáutica
dc.contributorOpen University
dc.contributorService de Physique Nucléaire
dc.contributorUniversidade Estadual Paulista (Unesp)
dc.contributorUniversidade de São Paulo (USP)
dc.date.accessioned2014-05-27T11:22:26Z
dc.date.accessioned2022-10-05T18:06:27Z
dc.date.available2014-05-27T11:22:26Z
dc.date.available2022-10-05T18:06:27Z
dc.date.created2014-05-27T11:22:26Z
dc.date.issued2007-03-26
dc.identifierAIP Conference Proceedings, v. 884, p. 118-122.
dc.identifier0094-243X
dc.identifier1551-7616
dc.identifierhttp://hdl.handle.net/11449/69578
dc.identifier10.1063/1.2710566
dc.identifier2-s2.0-33947387029
dc.identifier2-s2.0-33947387029.pdf
dc.identifier2914838355690793
dc.identifier0000-0002-3024-2671
dc.identifier.urihttp://repositorioslatinoamericanos.uchile.cl/handle/2250/3919002
dc.description.abstractWe analyze the surface geometry of the spherical even-even Ca, Ni, Sn and Pb nuclei using two approaches: The relativistic Dirac-Hartree-Bogoliubov one with several parameter sets and the non-relativistic Hartree-Fock-Bogoliubov one with the Gogny force. The proton and neutron density distributions are fitted to two-parameter Fermi density distributions to obtain the half-density radii and diffuseness parameters. Those parameters allow us to determine the nature of the neutron skins predicted by the models. The calculations are compared with existing experimental data. © 2007 American Institute of Physics.
dc.languageeng
dc.relationAIP Conference Proceedings
dc.rightsAcesso aberto
dc.sourceScopus
dc.subjectNuclear structure
dc.subjectRelativistic models
dc.subjectSurface geometry
dc.titleThe surface geometry of exotic nuclei
dc.typeTrabalho apresentado em evento


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