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dc.contributor.authorFrederico, T.-
dc.contributor.authorDelfino, A.-
dc.contributor.authorTomio, Lauro-
dc.contributor.authorYamashita, Marcelo Takeshi-
dc.date.accessioned2013-09-30T18:55:18Z-
dc.date.accessioned2014-05-20T14:10:16Z-
dc.date.accessioned2016-10-25T17:20:56Z-
dc.date.available2013-09-30T18:55:18Z-
dc.date.available2014-05-20T14:10:16Z-
dc.date.available2016-10-25T17:20:56Z-
dc.date.issued2012-10-01-
dc.identifierhttp://dx.doi.org/10.1016/j.ppnp.2012.06.001-
dc.identifier.citationProgress In Particle and Nuclear Physics. Amsterdam: Elsevier B.V., v. 67, n. 4, p. 939-994, 2012.-
dc.identifier.issn0146-6410-
dc.identifier.urihttp://hdl.handle.net/11449/24285-
dc.identifier.urihttp://acervodigital.unesp.br/handle/11449/24285-
dc.description.abstractThe theoretical status on universal aspects of weakly-bound neutron-rich light nuclei are reviewed, considering few-body approaches. We focus the review on the low-energy properties of light halo nuclei that can be treated within two- and three-body approaches (with one- and two-neutron halos), which are dominated by s-wave two-body interactions. The representative works studying the large two-neutron halos in light exotic nuclei with short-range interactions show that the general properties associated with the halo neutrons are model independent.and obey scaling laws, which are functions of the low-energy observables of the neutron-neutron and neutron-core subsystems, with one additional scale that represents the physics of the three-body system at short-ranges. The scaling laws for the s-wave two-neutron halos are identified with limit-cycles in a renormalized zero-range three-body model. The necessary basic concepts for interpreting the physics of large halos, and also to treat the zero-range interaction in few-body systems, are given. (c) 2012 Elsevier B.V. All rights reserved.en
dc.description.sponsorshipFundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)-
dc.description.sponsorshipConselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq)-
dc.format.extent939-994-
dc.language.isoeng-
dc.publisherElsevier B.V.-
dc.sourceWeb of Science-
dc.subjectHalo nucleien
dc.subjectFew-body systemsen
dc.subjectBinding energies and massesen
dc.subjectFaddeev equationen
dc.titleUniversal aspects of light halo nucleien
dc.typeoutro-
dc.contributor.institutionInstituto Tecnológico de Aeronáutica (ITA)-
dc.contributor.institutionUniversidade Federal Fluminense (UFF)-
dc.contributor.institutionUniversidade Estadual Paulista (UNESP)-
dc.description.affiliationInst Tecnol Aeronaut, Dept Fis, BR-12228900 Sao Jose Dos Campos, SP, Brazil-
dc.description.affiliationUniv Fed Fluminense, Inst Fis, BR-24210346 Niteroi, RJ, Brazil-
dc.description.affiliationUniv Estadual Paulista, Inst Fis Teor, BR-01140070 São Paulo, Brazil-
dc.description.affiliationUnespUniv Estadual Paulista, Inst Fis Teor, BR-01140070 São Paulo, Brazil-
dc.identifier.doi10.1016/j.ppnp.2012.06.001-
dc.identifier.wosWOS:000308630000003-
dc.rights.accessRightsAcesso restrito-
dc.relation.ispartofProgress in Particle and Nuclear Physics-
Appears in Collections:Artigos, TCCs, Teses e Dissertações da Unesp

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