Shell structure of potassium isotopes deduced from their magnetic moments
J. Papuga, M.L. Bissell, K. Kreim, C. Barbieri, K. Blaum, and M. De Rydt, T. Duguet, R.F. Garcia Ruiz, H. Heylen, M., Kowalska, R. Neugart, G. Neyens, W. Nortershauser, M.M. Rajabali, and R. Sanchez, N. Smirnova, V. Soma, D.T. Yordanov

TL;DR
This study investigates the nuclear structure of potassium isotopes beyond the N=28 shell gap by measuring their magnetic moments and spins, comparing results with shell-model calculations to understand wave function compositions.
Contribution
It provides new experimental data on ground-state spins and magnetic moments of K isotopes from N=19 to N=32, and analyzes the evolution of shell gaps using both shell-model and ab initio frameworks.
Findings
Dominant wave function component for odd-A isotopes up to 45K is a π 1d3/2^{-1} hole.
For 47K and 49K, the main component is a π 2s1/2^{-1} hole, reverting to π 1d3/2^{-1} in 51K.
Ground state of 48K is significantly mixed, leading to a 1− state; 50K has a 0− ground state with specific proton-neutron configurations.
Abstract
\item[Background] Ground-state spins and magnetic moments are sensitive to the nuclear wave function, thus they are powerful probes to study the nuclear structure of isotopes far from stability. \item[Purpose] Extend our knowledge about the evolution of the and states for K isotopes beyond the shell gap. \item[Method] High-resolution collinear laser spectroscopy on bunched atomic beams. \item[Results] From measured hyperfine structure spectra of K isotopes, nuclear spins and magnetic moments of the ground states were obtained for isotopes from up to . In order to draw conclusions about the composition of the wave functions and the occupation of the levels, the experimental data were compared to shell-model calculations using SDPF-NR and SDPF-U effective interactions. In addition, a detailed discussion about the evolution of the gap between…
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