Observational analysis demonstrates the role of isospin asymmetry in NN effective interaction, highlighting its significance in nucleon scattering.
We have investigated the role of isospin asymmetry of the NN effective interaction in the context of NA elastic scattering. To this purpose we represent the in-medium g matrix as an admixture of isospin-symmetric nuclear matter and pure neutron matter solutions of Brueckner-Hartree-Fock equations for infinite nuclear matter, denoted as g[ρ,β]. We use the Argonne v₁₈ bare potential to represent the NN interaction in free space, due to its ability to describe the NN scattering amplitudes up to 350 MeV. The density-dependent isospin-asymmetric g matrices are then used to calculate optical model potentials for elastic nucleon scattering off closed-shell nuclei. For this aim, we make use of the Arellano-Bauge δg-folding approach suited for an explicit treatment of nonlocal density matrices. This approach allows one to account for the local isospin-asymmetry and density dependence of the in-medium NN interaction. The resulting optical potentials are nonlocal since the entire nonlocal structure of the g matrix is retained. We observe that including the isospin asymmetry in the g matrix allows for a reasonable description of differential cross sections at nucleon beam energies between 40 and 200 MeV. In the case of proton scattering at energies below ≈65 MeV, at momentum transfers q below ≈10.28em0exfm^-1, the inclusion of neutronic-matter g matrices yields better agreement with the data as compared to the case when symmetric nuclear matter g matrices are used. These results provide evidence that the isospin-asymmetry in the NN effective interaction yield non-negligible effects in nucleon scattering off isospin-asymmetric targets at beam energies below 65 MeV.
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Fuentealba-Bustamante et al. (2025) studied this question.
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