R. de Groote

Novel Penning-trap techniques reveal isomeric states in $^{128}$In and $^{130}$In for the first time

D. A. Nesterenko, A. Kankainen, J. Kostensalo, C. R. Nobs, A. M. Bruce, O. Beliuskina, L. Canete, T. Eronen, E. R. Gamba, S. Geldhof, R. de Groote, A. Jokinen, J. Kurpeta, I. D. Moore, L. Morrison, Zs. Podolyák, I. Pohjalainen [1], S. Rinta-Antila [1], A. de Roubin [1], M. Rudigier [1], J. Suhonen [1], M. Vilén, V. Virtanen [1], J. Äystö

Abstract

Isomeric states in $^{128}$In and $^{130}$In have been studied with the JYFLTRAP Penning trap at the IGISOL facility. By employing novel ion manipulation techniques, different states were separated and masses of six beta-decaying states were measured. JYFLTRAP was also used to select the ions of interest for identification at a post-trap decay spectroscopy station. A new beta-decaying high-spin isomer feeding the $15^-$ isomer in $^{128}$Sn has been discovered in $^{128}$In at $1797.6(20)$ keV. Shell-model calculations employing a CD-Bonn potential re-normalized with the perturbative G-matrix approach suggest this new isomer to be a $16^+$ spin-trap isomer. In $^{130}$In, the lowest-lying $(10^-)$ isomeric state at $58.6(82)$ keV was resolved for the first time using the phase-imaging ion cyclotron resonance technique. The energy difference between the $10^-$ and $1^-$ states in $^{130}$In, stemming from parallel/antiparallel coupling of $(π0g_{9/2}^{-1})\otimes(ν0h_{11/2}^{-1})$, has been found to be around 200 keV lower than predicted by the shell model. Precise information on the energies of the excited states determined in this work is crucial for producing new improved effective interactions for the nuclear shell model description of nuclei near $^{132}$Sn.

Exploring the mass surface near the rare-earth abundance peak via precision mass measurements at JYFLTRAP

M. Vilen [1,2], J. M. Kelly, A. Kankainen [1], M. Brodeur [2], A. Aprahamian [2], L. Canete [1], R. de Groote [1], A. de Roubin [1], T. Eronen [1], A. Jokinen [1,3], I. D. Moore, M. R. Mumpower, D. A. Nesterenko, J. O'Brien, A. Pardo Perdomo [2,1], H. Penttilä, M. Reponen [1], S. Rinta-Antila [1], R. Surman [2]

Abstract

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, $^{161}$Pm, $^{163}$Sm, $^{164,165}$Eu, $^{167}$Gd, and $^{165,167,168}$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 $A\approx165$.

A new off-line ion source facility at IGISOL

M. Vilén, L. Canete, B. Cheal, A. Giatzoglou, R. de Groote, A. de Roubin, T. Eronen, S. Geldhof, A. Jokinen, A. Kankainen, I. D. Moore, D. A. Nesterenko, H. Penttilä, I. Pohjalainen [1], M. Reponen [1], S. Rinta-Antila [1]

Abstract

An off-line ion source station has been commissioned at the IGISOL (Ion Guide Isotope Separator On-Line) facility. It offers the infrastructure needed to produce stable ion beams from three off-line ion sources in parallel with the radioactive ion beams produced from the IGISOL target chamber. This has resulted in improved feasibility for new experiments by offering reference ions for Penning-trap mass measurements, laser spectroscopy and atom trap experiments.