𝔖 Bobbio Scriptorium
✦   LIBER   ✦

Optimization of relativistic mean field model for finite nuclei to neutron star matter

✍ Scribed by B.K. Agrawal; A. Sulaksono; P.-G. Reinhard

Book ID
113826295
Publisher
Elsevier Science
Year
2012
Tongue
English
Weight
555 KB
Volume
882
Category
Article
ISSN
0375-9474

No coin nor oath required. For personal study only.

πŸ“œ SIMILAR VOLUMES

Relativistic chiral mean field model for
Relativistic chiral mean field model for finite nuclei
✍ H. Toki; Y. Ogawa; S. Tamenaga; A. Haga πŸ“‚ Article πŸ“… 2007 πŸ› Elsevier Science 🌐 English βš– 782 KB

We study the role of pion for the structure of finite nuclei. We take the chiral sigma model, where the pions are the Nambu-Goldstone bosons of the chiral symmetry breaking. We then take the finite pion mean field in the relativistic mean field approximation. We study first the nuclei in the range o

Relativistic chiral mean field model for
Relativistic chiral mean field model for finite nuclei
✍ Yoko Ogawa; Hiroshi Toki πŸ“‚ Article πŸ“… 2011 πŸ› Elsevier Science 🌐 English βš– 405 KB

We present a method for proper treatment of pion-exchange interaction in the nuclear many-body problem in a relativistic chiral mean field (RCMF) model. The pionic correlation is expressed in 2-particle 2-hole (2p-2h) states in addition to the standard mean field state, to describe the full strength