2024/12/04 by Giuliani, Samuel A., Martínez-Pinedo, Gabriel, Bauswein, Andreas +1
#FOS: Physical sciences #High Energy Astrophysical Phenomena (astro-ph.HE) #Nuclear Theory (nucl-th)
paper · doi:10.48550/arxiv.2412.03243
Decomposing theoretical nuclear mass predictions into a liquid-drop parametrization and local shell effects shows that r-process abundances are virtually insensitive to large variations of the masses which originate from nuclear bulk properties of the model, such as the symmetry energy. Therefore, experimental and theoretical studies of masses devoted to r-process applications, such as the nucleosynthesis in the ejecta of neutron star mergers, should focus on the physical origin of local changes in mass trends without necessarily providing highly accurate mass determinations of individual nuclei.