r-Process Nucleosynthesis With Ab Initio Nuclear Masses Around The N=82 Shell Closure
This study demonstrates that ab initio nuclear mass calculations using the valence-space in-medium similarity renormalization group can refine r-process nucleosynthesis predictions around the N=82 shell closure, revealing a strengthened waiting point that slows the nucleosynthesis flow and significantly alters the abundance patterns of heavy elements compared to phenomenological models.