The surface geometry of exotic nuclei

dc.contributorUniversidade Estadual Paulista (UNESP)
dc.creatorCarlson, B. V.
dc.creatorBaldini-Neto, E.
dc.creatorHirata, D.
dc.creatorPéru-Desenfants, S.
dc.creatorBerger, J. F.
dc.creatorDe Conti, C.
dc.creatorChamon, L. C.
dc.date2014-05-27T11:22:26Z
dc.date2016-10-25T18:23:41Z
dc.date2014-05-27T11:22:26Z
dc.date2016-10-25T18:23:41Z
dc.date2007-03-26
dc.date.accessioned2017-04-06T01:24:11Z
dc.date.available2017-04-06T01:24:11Z
dc.identifierAIP Conference Proceedings, v. 884, p. 118-122.
dc.identifier0094-243X
dc.identifier1551-7616
dc.identifierhttp://hdl.handle.net/11449/69578
dc.identifierhttp://acervodigital.unesp.br/handle/11449/69578
dc.identifier10.1063/1.2710566
dc.identifier2-s2.0-33947387029.pdf
dc.identifier2-s2.0-33947387029
dc.identifierhttp://dx.doi.org/10.1063/1.2710566
dc.identifier.urihttp://repositorioslatinoamericanos.uchile.cl/handle/2250/890803
dc.descriptionWe 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.rightsinfo:eu-repo/semantics/closedAccess
dc.subjectNuclear structure
dc.subjectRelativistic models
dc.subjectSurface geometry
dc.titleThe surface geometry of exotic nuclei
dc.typeOtro


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