EXOTIC CARBON SYSTEMS IN TWO-NEUTRON HALO THREE-BODY MODELS

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dc.contributor.authorTomio, Lauro [UNESP]
dc.contributor.authorDelfino, Antonio
dc.contributor.authorFrederico, Tobias
dc.contributor.authorHadizadeh, M. R. [UNESP]
dc.contributor.authorYamashita, Marcelo Takeshi [UNESP]
dc.contributor.authorMarques de Carvalho, Raquel S.
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.date.accessioned2013-09-30T18:55:28Z
dc.date.accessioned2014-05-20T14:10:21Z
dc.date.available2013-09-30T18:55:28Z
dc.date.available2014-05-20T14:10:21Z
dc.date.issued2011-12-01
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.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.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.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.doi10.1142/S0218301311040335
dc.identifier.issn0218-3013
dc.identifier.lattes3740639726545315
dc.identifier.lattes8621258845956348
dc.identifier.urihttp://hdl.handle.net/11449/24292
dc.identifier.wosWOS:000298820900034
dc.language.isoeng
dc.publisherWorld Scientific Publ Co Pte Ltd
dc.relation.ispartofInternational Journal of Modern Physics E-nuclear Physics
dc.relation.ispartofjcr1.615
dc.relation.ispartofsjr0,687
dc.rights.accessRightsAcesso restrito
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.typeArtigo
dcterms.licensehttp://www.worldscientific.com/page/authors/author-rights
dcterms.rightsHolderWorld Scientific Publ Co Pte Ltd
unesp.author.lattes3740639726545315
unesp.author.lattes8621258845956348
unesp.author.orcid0000-0002-2559-092X[5]
unesp.campusUniversidade Estadual Paulista (Unesp), Instituto de Física Teórica (IFT), São Paulopt

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São Paulo - IFT - Instituto de Física Teórica