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Nuclei, superheavy nuclei, and hypermatter in a chiral SU(3) model

  • 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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Metadaten
Verfasserangaben:Christian Beckmann, Panajotis Papazoglou, Detlef ZschiescheGND, Stefan SchrammGND, Horst StöckerORCiDGND, Walter GreinerGND
URN:urn:nbn:de:hebis:30-21497
Dokumentart:Preprint
Sprache:Englisch
Datum der Veröffentlichung (online):17.11.2005
Jahr der Erstveröffentlichung:2001
Veröffentlichende Institution:Universitätsbibliothek Johann Christian Senckenberg
Datum der Freischaltung:17.11.2005
Freies Schlagwort / Tag:Hypermaterie; Kerne; SU (3) - Symmetrie; superschwer
SU(3)-symmetry; hypermatter; nuclei; superheavy
Quelle:Phys.Rev.C65:024301,2002. [nucl-th/0106014]
HeBIS-PPN:185535429
Institute:Physik / Physik
DDC-Klassifikation:5 Naturwissenschaften und Mathematik / 53 Physik / 530 Physik
Lizenz (Deutsch):License LogoDeutsches Urheberrecht