Shell structure of potassium isotopes deduced from their magnetic moments

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. Purpose: Extend our knowledge about the evolution of the 1/2+ and 3/2+ states for K isotopes beyond the N = 28 shell gap. Method: High-resolution collinear laser spectroscopy on bunched atomic beams. Results: From measured hyperfine structure spectra of K isotopes, nuclear spins, and magnetic moments of the ground states were obtained for isotopes from N = 19 up to N = 32. 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 proton 1d3/2 and 2s1/2 in the shell model and ab initio framework is also presented. Conclusions: The dominant component of the wave function for the odd-A isotopes up to 45K is a π1d−1_{3/2} hole. For 47,49K, the main component originates from a π2s−1_{1/2} hole configuration and it inverts back to the π1d−1_{3/2} in 51K. For all even-A isotopes, the dominant configuration arises from a π1d−1_{3/2} hole coupled to a neutron in the ν1f7/2 or ν2p3/2 orbitals. Only for 48K, a significant amount of mixing with π2s−1_{1/2}⊗ ν(pf ) is observed leading to a I^π = 1− ground state. For 50K, the ground-state spin-parity is 0− with leading configuration π1d−1_{3/2}⊗ ν2p−1_{3/2}.12 pages, 10 figures, 7 tablesstatus: publishe