Pairing gap energy correction in Shell model for the neutron-rich tin isotopes



Título del documento: Pairing gap energy correction in Shell model for the neutron-rich tin isotopes
Revista: Brazilian journal of physics
Base de datos: PERIÓDICA
Número de sistema: 000329409
ISSN: 0103-9733
Autors: 1
1
1
Institucions: 1Mentouri-Constantine University, Mathematic and Subatomic Physics Laboratory, Constantine. Argelia
Any:
Període: Dic
Volum: 39
Número: 4
Paginació: 663-666
País: Brasil
Idioma: Inglés
Tipo de documento: Artículo
Enfoque: Experimental
Resumen en inglés The region in the vicinity of 132Sn, gathering numerous isotopes of important masses, shows lots of interests for explaining the most interesting phenomena. It offers among others the possibility to extract the N-N empirical interactions so as to test theoretical shell model description of nuclear structure in this region. The researches on the neutron-rich tin isotopes present the anomalies in a systematic variation on various spectroscopic data such as the first 2+ excited state and reduced probabilities B(E2;2+→ 0+). In order to improve the OXBASH interactions which are based on the shell model calculations, we have modified some neutron-neutron and proton-proton tow body matrix elements of CW5082 interaction of 132Sn region by adding to them the pairing gap energy. The calculations turn out a new interaction so called CWΔ5082, allowing to determine the excited energies and the reduced probabilities B(E2) of Sn and Te isotopes for A = 134 and 136 masses. The obtained results display a remarkable enhancement in the predictive power of experimental values
Disciplines Física y astronomía
Paraules clau: Física,
Física nuclear,
Región Sn132,
Código Oxbash,
Interacciones efectivas
Keyword: Physics and astronomy,
Nuclear physics,
Physics,
132Sn region,
Oxbash code,
Effective interaction
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