Probing the N=104 midshell region for the r process via precision mass spectrometry of neutron-rich rare-earth isotopes with the JYFLTRAP double Penning trap
A. Jaries🇫🇮 · S. Nikas🇫🇮 · A. Kankainen🇫🇮 · T. Eronen🇫🇮 · O. Beliuskina🇫🇮 · T. Dickel🇩🇪 · M. Flayol🇫🇷 · Z. Ge🇫🇮 · M. Hukkanen🇫🇮 · M. Mougeot🇫🇮 · I. Pohjalainen🇫🇮 · A. Raggio🇫🇮 and 4 other authors
We have performed high-precision mass measurements of neutron-rich rare-earth Tb, Dy and Ho isotopes using the Phase-Imaging Ion-Cyclotron-Resonance technique at the JYFLTRAP double Penning trap. We report on the first experimentally determined mass values for Tb, Dy and Dy, as well as the first high-precision mass measurements of Dy and Ho. For Ho, the two long-lived ground and isomeric states were resolved and their mass measured, yielding an isomer excitation energy of ~keV. In addition, we have performed independent crosschecks of previous Penning-trap values obtained for Tb and Dy. We have extended the systematics of two-neutron separation energies to the neutron midshell at in all of the studied isotopic chains. Our updated and new mass measurements provide better mass-related constraints for the neutron-capture reaction rates relevant to the astrophysical rapid neutron capture (r) process. The r-process abundances calculated with the new mass values seem to produce a steeper minimum at A=170 and differ by around 15-30\% from the abundances computed with the Atomic Mass Evaluation 2020 values.