Nuclei, Superheavy Nuclei and Hypermatter in a chiral SU(3)-Modell

Details Nuclei, Superheavy Nuclei and Hypermatter in a chiral SU(3)-Modell Nuclei, Superheavy Nuclei and Hypermatter in a chiral SU(3)-Modell

2001-06-06

arxiv.org/abs/nucl-th/0106014v1

Phys.Rev. C65 (2002) 024301

Physics

Nuclear Physics

Nuclear Theory

19 pages, 11 figures

Scientific paper

10.1103/PhysRevC.65.024301

A model based on chiral SU(3)-symmetry in nonlinear realisation is used for the investigation of nuclei, superheavy nuclei, hypernuclei and multistrange nuclear objects (so called MEMOs). The model works very well in the case of nuclei and hypernuclei with one Lambda-particle and rules out MEMOs. Basic observables which are known for nuclei and hypernuclei are reproduced satisfactorily. The model predicts Z=120 and N=172, 184 and 198 as the next shell closures in the region of superheavy nuclei. The calculations have been performed in self-consistent relativistic mean field approximation assuming spherical symmetry. The parameters were adapted to known nuclei.

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