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Please use this identifier to cite or link to this item: http://acervodigital.unesp.br/handle/11449/24292
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dc.contributor.authorTomio, Lauro-
dc.contributor.authorDelfino, Antonio-
dc.contributor.authorFrederico, Tobias-
dc.contributor.authorHadizadeh, M. R.-
dc.contributor.authorYamashita, Marcelo Takeshi-
dc.contributor.authorMarques de Carvalho, Raquel S.-
dc.date.accessioned2013-09-30T18:55:28Z-
dc.date.accessioned2014-05-20T14:10:21Z-
dc.date.accessioned2016-10-25T17:21:04Z-
dc.date.available2013-09-30T18:55:28Z-
dc.date.available2014-05-20T14:10:21Z-
dc.date.available2016-10-25T17:21:04Z-
dc.date.issued2011-12-01-
dc.identifierhttp://dx.doi.org/10.1142/S0218301311040335-
dc.identifier.citationInternational Journal of Modern Physics E-nuclear Physics. Singapore: World Scientific Publ Co Pte Ltd, v. 20, p. 254-262, 2011.-
dc.identifier.issn0218-3013-
dc.identifier.urihttp://hdl.handle.net/11449/24292-
dc.identifier.urihttp://acervodigital.unesp.br/handle/11449/24292-
dc.description.abstractThe general properties of exotic carbon systems, considered as a core with a two-neutron (n - n) halo, are described within a renormalized zero-range three-body model. In particular, it is addressed the cases with a core of (18)C and (20)C. In such a three-body framework, (20)C has a bound subsystem ((19)C), whereas (22)C has a Borromean structure with all subsystems unbound. (22)C is also known as the heaviest:, carbon halo nucleus discovered. The spatial distributions of such weakly-bound three-body systems are studied in terms of a universal scaling function, which depends on the mass ratio of the particles, as well as on the nature of the subsystems.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.extent254-262-
dc.language.isoeng-
dc.publisherWorld Scientific Publ Co Pte Ltd-
dc.sourceWeb of Science-
dc.subjectHalo nucleien
dc.subjectBinding Energiesen
dc.subjectFaddeev Equationen
dc.subjectThree-body Systemsen
dc.titleEXOTIC CARBON SYSTEMS IN TWO-NEUTRON HALO THREE-BODY MODELSen
dc.typeoutro-
dc.contributor.institutionUniversidade Estadual Paulista (UNESP)-
dc.contributor.institutionUniversidade Federal Fluminense (UFF)-
dc.contributor.institutionInstituto Tecnológico de Aeronáutica (ITA)-
dc.contributor.institutionUniversidade Federal de São Paulo (UNIFESP)-
dc.description.affiliationUniv Estadual Paulista, Inst Fis Teor, BR-01140070 São Paulo, Brazil-
dc.description.affiliationUniv Fed Fluminense, Inst Fis, BR-24210346 Niteroi, RJ, Brazil-
dc.description.affiliationInst Tecnol Aeronaut, Dept Fis, BR-12228900 Sao Jose Dos Campos, SP, Brazil-
dc.description.affiliationUniv Fed São Paulo, BR-04039002 São Paulo, Brazil-
dc.description.affiliationUnespUniv Estadual Paulista, Inst Fis Teor, BR-01140070 São Paulo, Brazil-
dc.identifier.doi10.1142/S0218301311040335-
dc.identifier.wosWOS:000298820900034-
dc.rights.accessRightsAcesso restrito-
dc.relation.ispartofInternational Journal of Modern Physics E-nuclear Physics-
Appears in Collections:Artigos, TCCs, Teses e Dissertações da Unesp

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