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Precise knowledge about nuclear symmetry energy can be tentatively calibratedthrough multimessenger constraints. Neutron skin thickness (NST) of a heavynucleus has been known as one of the most sensitive indicators to probe theisovector components of effective interactions in asymmetric nuclear matter.Recent studies suggest that the experimental data coming from the CREX andPREX2 Collaborations are not mutually compatible within the existing nuclearmodels. We further review the quantification of the slope parameter of symmetryenergy $L$ from the neutron skin thicknesses of $^{48}$Ca and $^{208}$Pb. TheSkyrme energy density functionals (EDFs) classified by various isoscalarincompressibility coefficients $K$ are employed to evaluate the bulk propertiesof finite nuclei. The calculated results suggest that the slope parameter $L$deduced from $^{208}$Pb is sensitive to the compression modulus of symmetricnuclear matter, but not in $^{48}$Ca. The effective parameter sets classifiedby $K=220$ MeV can almost give a overlap range of $L$ from $^{48}$Ca and$^{208}$Pb.

Quantification of symmetry energy with the isoscalar nuclear matter property