Differential analysis of incompressibility in neutron-rich nuclei
arXiv:2102.10683 · doi:10.1103/PhysRevC.104.034610
Abstract
Both the incompressibility \Ka of a finite nucleus of mass A and that () of infinite nuclear matter are fundamentally important for many critical issues in nuclear physics and astrophysics. While some consensus has been reached about the , accurate theoretical predictions and experimental extractions of characterizing the isospin dependence of \Ka have been very difficult. We propose a differential approach to extract the \Kt and \Ki independently from the \Ka data of any two nuclei in a given isotope chain. Applying this new method to the \Ka data from isoscalar giant monopole resonances (ISGMR) in even-even Pb, Sn, Cd and Ca isotopes taken by U. Garg {\it et al.} at the Research Center for Nuclear Physics (RCNP), Osaka University, Japan, we find that the Cd-Cd and Sn-Sn pairs having the largest differences in isospin asymmetries in their respective isotope chains measured so far provide consistently the most accurate up-to-date \Kt value of MeV and MeV, respectively, largely independent of the remaining uncertainties of the surface and Coulomb terms in expanding the , while the values extracted from different isotopes chains are all well within the current uncertainty range of the community consensus for . Moreover, the size and origin of the "Soft Sn Puzzle" is studied with respect to the "Stiff Pb Phenomenon". It is found that the latter is favored due to a much larger (by MeV) \Kt for Pb isotopes than for Sn isotopes, while the \Ki from analyzing the \Ka data of Sn isotopes is only about 5 MeV less than that from analyzing the Pb data.
More discussions added. Phys. Rev. C in press
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