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dc.creatorChen, Lie-Wen
dc.creatorCai, Bao-Jun
dc.creatorKo, Che Ming
dc.creatorLi, Bao-An
dc.creatorShen, Chun
dc.creatorXu, Jun.
dc.date.accessioned2011-09-13T21:26:48Z
dc.date.available2011-09-13T21:26:48Z
dc.date.issued2009
dc.identifier.citationLie-Wen Chen, Bao-Jun Cai, Che Ming Ko, Bao-An Li, Chun Shen and Jun Xu. Phys.Rev.C 80 014322 2009. "Copyright (2009) by the American Physical Society."en
dc.identifier.urihttp://dx.doi.org/10.1103/PhysRevC.80.014322
dc.identifier.urihttp://hdl.handle.net/1969.1/127084
dc.descriptionJournals published by the American Physical Society can be found at http://publish.aps.org/en
dc.description.abstractAnalytical expressions for the saturation density of asymmetric nuclear matter as well as its binding energy and incompressibility at saturation density are given up to fourth order in the isospin asymmetry delta=(rho(n)-rho(p))/rho using 11 characteristic parameters defined by the density derivatives of the binding energy per nucleon of symmetric nuclear matter, the symmetry energy E(sym) (rho), and the fourth-order symmetry energy E(sym,4)(rho) at normal nuclear density rho(0). Using an isospin- and momentum-dependent modified Gogny interaction (MDI) and the Skyrme-Hartree-Fock (SHF) approach with 63 popular Skyrme interactions, we have systematically studied the isospin dependence of the saturation properties of asymmetric nuclear matter, particularly the incompressibility K(sat)(delta)=K(0)+K(sat,2)delta(2)+K(sat,4)delta(4)+O(delta(6)) at saturation density. Our results show that the magnitude of the higher order K(sat,4) parameter is generally small compared to that of the K(sat,2) parameter. The latter essentially characterizes the isospin dependence of the incompressibility at saturation density and can be expressed as K(sat,2)=K(sym)-6L-J(0)K(0)L, where L and K(sym) represent, respectively, the slope and curvature parameters of the symmetry energy at rho(0) and J(0) is the third-order derivative parameter of symmetric nuclear matter at rho(0). Furthermore, we have constructed a phenomenological modified Skyrme-like (MSL) model that can reasonably describe the general properties of symmetric nuclear matter and the symmetry energy predicted by both the MDI model and the SHF approach. The results indicate that the higher order J(0) contribution to K(sat,2) generally cannot be neglected. In addition, it is found that there exists a nicely linear correlation between K(sym) and L as well as between J(0)/K(0) and K(0). These correlations together with the empirical constraints on K(0),L,E(sym) (rho(0)), and the nucleon effective mass lead to an estimate of K(sat,2)=-370 +/- 120 MeV.en
dc.language.isoen
dc.publisherAmerican Physical Society
dc.subjectHEAVY-ION COLLISIONSen
dc.subjectBOGOLiuBOV MASS FORMULASen
dc.subjectGIANT MONOPOLEen
dc.subjectRESONANCEen
dc.subjectNEUTRON-STAR STRUCTUREen
dc.subjectEQUATION-OF-STATEen
dc.subjectSYMMETRY ENERGYen
dc.subjectEXOTIC NUCLEIen
dc.subjectMEAN-FIELDen
dc.subjectSKYRME PARAMETRIZATIONen
dc.subjectINTERMEDIATE ENERGIESen
dc.subjectPhysicsen
dc.titleHigher-order effects on the incompressibility of isospin asymmetric nuclear matteren
dc.typeArticleen
local.departmentPhysics and Astronomyen


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