Properties of N∗(1535) at finite density
✍
Hungchong Kim; D. Jido; M. Oka
📂
Article
📅
1998
🏛
Elsevier Science
🌐
English
⚖ 628 KB
We improve so-called "naive" and "mirror" models for the positive and negative parity nucleons, N and N\*, by introducing non-linear terms allowed by chiral symmetry. Both models in this improvement reproduce the observed nucleon axial charge in free space and reveal interesting density dependence o