Radii in weakly-bound light halo nuclei

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dc.contributor.authorYamashita, Marcelo Takeshi [UNESP]
dc.contributor.authorTomio, L.
dc.contributor.authorFrederico, T.
dc.contributor.institutionUniversidade Estadual Paulista (Unesp)
dc.contributor.institutionUniversidade de São Paulo (USP)
dc.contributor.institutionCtr Aerosp Technol
dc.date.accessioned2014-05-20T14:05:40Z
dc.date.available2014-05-20T14:05:40Z
dc.date.issued2004-04-19
dc.description.abstractA systematic study of the root-mean-square distance between the constituents of weakly-bound nuclei consisting of two halo neutrons and a core is performed using a renormalized zero-range model. The radii are obtained from a universal scaling function that depends on the mass ratio of the neutron and the core, as well as on the nature of the subsystems, bound or virtual. Our calculations are qualitatively consistent with recent data for the neutron-neutron root-mean-square distance in the halo of Li-11 and Be-14 nuclei. (C) 2004 Published by Elsevier B.V.en
dc.description.affiliationUniv Estadual Paulista, Inst Fis Teor, BR-01405900 São Paulo, Brazil
dc.description.affiliationUniv São Paulo, Inst Fis, Lab Acelerador Linear, BR-05315970 São Paulo, Brazil
dc.description.affiliationCtr Aerosp Technol, Inst Tecnol Aeronaut, Dept Fis, BR-12228900 Sao Jose Dos Campos, Brazil
dc.description.affiliationUnespUniv Estadual Paulista, Inst Fis Teor, BR-01405900 São Paulo, Brazil
dc.format.extent40-54
dc.identifierhttp://dx.doi.org/10.1016/j.nuclphysa.2004.02.003
dc.identifier.citationNuclear Physics A. Amsterdam: Elsevier B.V., v. 735, n. 1-2, p. 40-54, 2004.
dc.identifier.doi10.1016/j.nuclphysa.2004.02.003
dc.identifier.issn0375-9474
dc.identifier.lattes3740639726545315
dc.identifier.urihttp://hdl.handle.net/11449/23051
dc.identifier.wosWOS:000220645600003
dc.language.isoeng
dc.publisherElsevier B.V.
dc.relation.ispartofNuclear Physics A
dc.relation.ispartofjcr1.992
dc.relation.ispartofsjr0,938
dc.rights.accessRightsAcesso restrito
dc.sourceWeb of Science
dc.titleRadii in weakly-bound light halo nucleien
dc.typeArtigo
dcterms.licensehttp://www.elsevier.com/about/open-access/open-access-policies/article-posting-policy
dcterms.rightsHolderElsevier B.V.
unesp.author.lattes3740639726545315
unesp.author.orcid0000-0002-2559-092X[1]
unesp.campusUniversidade Estadual Paulista (Unesp), Instituto de Física Teórica (IFT), São Paulopt

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