Abstract

The incompressibility Ksat(δ)K_sat(δ) of isospin asymmetric nuclear matter at its saturation density. Our results show that in the expansion of Ksat(δ)K_sat(δ) in powers of isospin asymmetry δδ, i.e., Ksat(δ)K_sat(δ)=K_{0}+K_{sat,2}δ^{2}+K_{sat,4}δ^{4}+O(δ^{6})$, the magnitude of the 4th-order K_{sat,4} parameter is generally small. The 2nd-order K_{sat,2} parameter thus essentially characterizes the isospin dependence of the incompressibility of asymmetric nuclear matter at saturation density. Furthermore, the K_{sat,2} can be expressed as K_{sat,2}=K_{sym}-6L-J_{0}/{K_{0}L in terms of the slope parameter $Landthecurvatureparameter and the curvature parameter K_{\mathrm{sym}}ofthesymmetryenergyandthethird−orderderivativeparameter of the symmetry energy and the third-order derivative parameter J_0oftheenergyofsymmetricnuclearmatteratsaturationdensity,andwefindthehigherorder of the energy of symmetric nuclear matter at saturation density, and we find the higher order J_0contributiontoKsat,2generallycannotbeneglected.Also,wehavefoundalinearcorrelationbetweenKsymand contribution to K_{sat,2} generally cannot be neglected. Also, we have found a linear correlation between K_{sym} and Laswellasbetween as well as between J_{0}/K_{0}and and K_{0}.Usingthesecorrelationstogetherwiththeempiricalconstraintson. Using these correlations together with the empirical constraints on K_{0}and and L,thenuclearsymmetryenergy, the nuclear symmetry energy E_sym(ρ_{0})$ at normal nuclear density, and the nucleon effective mass, we have obtained an estimated value of K_{sat,2}=-370 +- 120 MeV for the 2nd-order parameter in the isospin asymmetry expansion of the incompressibility of asymmetric nuclear matter at its saturation density.

Explore this paper’s authors, topics and related work.

Building this map preview

BZPEER is loading the nearby papers, people, topics and institutions for this page.

Reviews 0

Write a reviewWrite

No reviews yet.

Discussion 0

Add a commentWrite

No comments yet.