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Isospin Constraints on the Parametric Coupling Model for Nuclear Matter
Authors: Guilherme F. Marranghello, Constança Providência e Alexandre M. S. Santos
Ref.: Phys. Rev. C 81, 024307-1-024307-1 (2010)
Abstract: We make use of isospin constraints to study the parametric coupling model and the properties of asymmetric nuclear matter. Besides the usual constraints for nuclear matter - effective nucleon mass and the incompressibility at saturation density - and the neutron star constraints - maximum mass and radius - we have studied the properties related with the symmetry energy. These properties have constrained to a small range the parameters of the model. We have applied our results to study the thermodynamic instabilities in the liquid-gas phase transition as well as the neutron star configurations.
