Exploring the mass surface near the rare-earth abundance peak via precision mass measurements at JYFLTRAP
M. Vilen🇫🇮 · J.M. Kelly🇫🇮 · A. Kankainen🇫🇮 · M. Brodeur🇺🇸 · A. Aprahamian🇺🇸 · L. Canete🇫🇮 · R. de Groote🇫🇮 · A. de Roubin🇫🇮 · T. Eronen🇫🇮 · A. Jokinen🇫🇮 · I.D. Moore🇫🇮 · M.R. Mumpower🇺🇸 and 7 other authors
The JYFLTRAP double Penning trap at the Ion Guide Isotope Separator On-Line (IGISOL) facility has been used to measure the atomic masses of 13 neutron-rich rare-earth isotopes. Eight of the nuclides, Pm, Sm, Eu, Gd, and Tb, were measured for the first time. The systematics of the mass surface has been studied via one- and two-neutron separation energies as well as neutron pairing-gap and shell-gap energies. The proton-neutron pairing strength has also been investigated. The impact of the new mass values on the astrophysical rapid neutron capture process has been studied. The calculated abundance distribution results in a better agreement with the solar abundance pattern near the top of the rare-earth abundance peak at around .