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


Autoria(s): Tomio, Lauro; Delfino, Antonio; Frederico, Tobias; Hadizadeh, M. R.; Yamashita, Marcelo Takeshi; Marques de Carvalho, Raquel S.
Contribuinte(s)

Universidade Estadual Paulista (UNESP)

Data(s)

30/09/2013

20/05/2014

30/09/2013

20/05/2014

01/12/2011

Resumo

Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)

Conselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq)

The 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.

Formato

254-262

Identificador

http://dx.doi.org/10.1142/S0218301311040335

International Journal of Modern Physics E-nuclear Physics. Singapore: World Scientific Publ Co Pte Ltd, v. 20, p. 254-262, 2011.

0218-3013

http://hdl.handle.net/11449/24292

10.1142/S0218301311040335

WOS:000298820900034

Idioma(s)

eng

Publicador

World Scientific Publ Co Pte Ltd

Relação

International Journal of Modern Physics E-nuclear Physics

Direitos

closedAccess

Palavras-Chave #Halo nuclei #Binding Energies #Faddeev Equation #Three-body Systems
Tipo

info:eu-repo/semantics/article