Relativistic Mean-Field Models and Nuclear Matter Constraints
arXiv:1303.2562 · doi:10.1063/1.4804125
Abstract
This work presents a preliminary study of 147 relativistic mean-field (RMF) hadronic models used in the literature, regarding their behavior in the nuclear matter regime. We analyze here different kinds of such models, namely: (i) linear models, (ii) nonlinear Ï^3+Ï^4 models, (iii) Ï^3+Ï^4+Ï^4 models, (iv) models containing mixing terms in the fields Ïand Ï, (v) density dependent models, and (vi) point-coupling ones. In the finite range models, the attractive (repulsive) interaction is described in the Lagrangian density by the Ï(Ï) field. The isospin dependence of the interaction is modeled by the Ïmeson field. We submit these sets of RMF models to eleven macroscopic (experimental and empirical) constraints, used in a recent study in which 240 Skyrme parametrizations were analyzed. Such constraints cover a wide range of properties related to symmetric nuclear matter (SNM), pure neutron matter (PNM), and both SNM and PNM.
3 Pages, submitted for proceedings of XXXV Reunião de Trabalho sobre FÃsica Nuclear no Brasil 2012