Speaker
Description
The rapid neutron capture process (r-process) is a key mechanism responsible for producing nearly half of the nuclei heavier than iron in explosive scenarios. In the solar-system abundance pattern, the Rare-Earth Peak (REP) around mass number $A = 160$ represents a significant feature resulting from freeze-out during the final stages of neutron exposure. The BRIKEN collaboration [1] conducted extensive measurements of $\beta$-decay properties of nuclei of interest to better understand the r-process at the Radioactive Isotope Beam Factory (RIBF), RIKEN Nishina Center, Japan. Our study focuses on the Barium to Neodymium region crucial for REP r-process nucleosynthesis [2,3]. In this contribution, we present the final experimental results from the BRIKEN-REP experiment, which yielded new $T_{1/2}$ and $P_{1n}$ branching ratios. Furthermore, we discuss the implications of these findings for global models of nuclear structure, aiming to refine theoretical predictions and enhance our understanding of REP r-process nucleosynthesis.
[1] J.L. Tain et. al , Acta Physica Polonica B {49(03), 417 $-$ 428 (2018).
[2] M. R. Mumpower et al , Phys. Rev. C 85, 045801 (2012).
[3] A. Arcones and G. Martinez Pinedo , Phys. Rev. C 83, 045809 (2011).