Nuclear matter incompressibility coefficient in relativistic and nonrelativistic microscopic models

Details Nuclear matter incompressibility coefficient in relativistic and nonrelativistic microscopic models Nuclear matter incompressibility coefficient in relativistic and nonrelativistic microscopic models

2003-08-14

arxiv.org/abs/nucl-th/0308042v1

Phys.Rev. C68 (2003) 031304

Physics

Nuclear Physics

Nuclear Theory

Revtex file (13 pages), appearing in PRC-Rapid Comm

Scientific paper

10.1103/PhysRevC.68.031304

We systematically analyze the recent claim that nonrelativistic and relativistic mean field (RMF) based random phase approximation (RPA) calculations for the centroid energy E_0 of the isoscalar giant monopole resonance yield for the nuclear matter incompressibility coefficient, K_{nm}, values which differ by about 20%. For an appropriate comparison with the RMF based RPA calculations, we obtain the parameters for the Skyrme force used in the nonrelativistic model by adopting the same procedure as employed in the determination of the NL3 parameter set of an effective Lagrangian used in the RMF model. Our investigation suggest that the discrepancy between the values of K_{nm} predicted by the relativistic and nonrelativistic models is significantly less than 20%.

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