Hypernuclei and nuclear matter in a chiral SU(3) RMF model
arXiv:nucl-th/0702008 · doi:10.1140/epja/i2007-10474-6
Abstract
We develop a chiral SU(3) RMF model for octet baryons, as an extension of the recently developed chiral SU(2) RMF model with logarithmic sigma potential. For Sigma-meson coupling, strong repulsion(SR) and weak repulsion(WR) cases are examined in existing atomic shift data of Sigma^-. In both of these cases, we need an attractive pocket of a few MeV depth around nuclear surface.
4 pages, 8 figures, to appear in the proceedings of the IX International Conference on Hypernuclear and Strange Particle Physics (HYP2006)
References in corpus (4)
Cited by in corpus (4)
- Tables of Hyperonic Matter Equation of State for Core-Collapse Supernovae
- Lambda hypernuclei and neutron star matter in a chiral SU(3) relativistic mean field model with a logarithmic potential
- Nuclear symmetry energy with mesonic cross-couplings in the effective chiral model
- Nuclear Matter and Finite Nuclei in the Effective Chiral Model