Bayesian Inference of the Symmetry Energy and the Neutron Skin in 48Ca and 208Pb from CREX and PREX-2

Abstract

Using the recent model-independent determination of the charge-weak form factor difference F CW in 48Ca and 208Pb by the CREX and PREX-2 collaborations together with some well-determined properties of doubly magic nuclei, we perform Bayesian inference of the symmetry energy E sym() and the neutron skin thickness r np of 48Ca and 208Pb within the Skyrme energy density functional (EDF). We find the inferred E sym() and r np separately from CREX and PREX-2 are compatible with each other at 90\% C.L., although they are inconsistent at 68.3\% C.L. with CREX (PREX-2) favoring a very soft (stiff) E sym() and rather small (large) r np. By combining the CREX and PREX-2 data, we obtain a soft symmetry energy around saturation density 0 and thinner r np of 48Ca and 208Pb, which are found to be closer to the corresponding results from CREX alone, implying the PREX-2 is less effective to constrain the E sym() and r np due to its lower precision of F CW. Furthermore, we find the Skyrme EDF results inferred by combining the CREX and PREX-2 data nicely agree with the measured dipole polarizabilities αD in 48Ca and 208Pb as well as the neutron matter equation of state from microscopic calculations. The implications of the inferred soft E sym() around 0 are discussed.

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