Abstract
According to the Hugenholtz–Van Hove theorem, the symmetry energy and its density slope can be decomposed uniquely in terms of the single-nucleon potential in asymmetric nuclear matter which, at normal density, can be constrained by the nucleon optical model potential extracted from analyzing the nucleon–nucleus scattering data. To more accurately extract information on the symmetry energy and its density slope at normal density from neutron–nucleus scattering data, going beyond the well-known Lane potential, we include consistently the second-order terms in isospin asymmetry in both the optical model potential and the symmetry energy decomposition. We find that the strength of the second-order symmetry potential Usym,2 in asymmetric nuclear matter is significant compared to the first-order one Usym,1, especially at high nucleon momentum. While the Usym,1 at normal density decreases with nucleon momentum, the Usym,2 is found to have the opposite behavior. Moreover, we discuss effects of the Usym,1 and Usym,2 on determining the density dependence of the symmetry energy, and we find that the available neutron–nucleus scattering data favor a softer density dependence of the symmetry energy at normal density with a negligible contribution from the Usym,2.
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